title (Result I)

Result of query: info cati 14 CMi|$ Pi Note:

Details on Acronym: 30 Dor
30 Dor	(30 Dor nebula)
*****	Avoid the usage of 30 Dor, prefer [KKB2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Pi		(Cyrillic letter for Parenago)	Pi = $Pi.
*****	Avoid the usage of Pi , prefer Parenago	Details on Acronym: *
*	(Star)= (BAYER) = (FLAMSTEED)
Write:	<<* A CCC>> <<* a CCC>> <<* ggg CCC>> <<* gggNN CCC>> <<* NNN CCC>>
Object:	* (SIMBAD class: Star)
Note:	In SIMBAD only. To find the designation as in the literature, drop the first word (*). For star names following the Bayer's Greek letter system and Flamsteed numbers.
Details on Acronym: **
**	(Double Star)
Write:	<< AAA NNNNAA>> << AAAA NNNAA>> << H N NNNAA>> << H N NNNAA>>
Object:	(SIMBAD class: = Double or Multiple Star)
Note:	In SIMBAD only. To find the designation as in the literature, drop the first word (**). 'AAA' is an abbreviation for discoverers' names. A list of these abbreviations can be found at : http://www.astro.gsu.edu/wds/Webtextfiles/wdsnewref.txt An additional 'A' is used to distinguish between systems from the main list or appendices from the same discoverer (e.g. STF 3136 is the 3136th system in Struve's main list, whereas STFA 11 and STFB 11 are the 11th system respectively in Struve's appendix I and II). For the William Herschel discoveries, a list identifier is added to column three of each designation. For example: H 19 (at 16 hours) was originally H II 19 and is now known as H 2 19, H 7 (at 18 hours) was originally H V 7 and is now known as H 5 7, and H 111 (at 06 hours) was originally H N 111 and is now known as H N 111.
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Note:	Atlas of the LMC. There are two sets of charts, one in V and one in B. Each set consists of about 80 charts of square areas measuring 1deg1/4 on a side. A master set shows their locations and interrelation, and Tables 3 and 4 give 1975 eq. coordinates of their centers. Table 12: see SV* HV.
Ref:	=1967SAOP.4699....1H
by	HODGE P.W. , WRIGHT F.W.
	SAO Publications, 4699, 1-None (1967)
	The Large Magellanic Cloud.
o	Atlas of the LMC.
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Auth.:	DIXON R.S.
=E=	Catalogue in electronic form as VII/2
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1970MmRAS..73..153W
by	WACKERLING L.R.
	Mem. R. Astron. Soc., 73, 153-319 (1970)
	A catalogue of early-type stars whose spectra have shown emission lines.
o	<Em* CDS NNNN> (Nos 1-5326).
Ref:	=1977PW&SO...2...71S
by	STEPHENSON C.B. , SANDULEAK N.
	Publ. Warner & Swasey Obs., 2, 71-None (1977)
	New position determinations, and other data, for 1280 known Hα-emission stars in the Milky Way.
=E=	Catalogue in electronic form as III/17
=E=	Catalogue in electronic form as <III/17B/>
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Auth.:	ABT H.A.+
Ref:	=1975BICDS...8...12B
by	BARBIER M.
	Bull. Inf. Centre Donnees Stellaires, 8, 12-None (1975)
	Radial velocities.
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1973ApJS...26...19V
by	VAN DEN BERGH S. , MARSCHER A.P., TERZIAN Y.
	Astrophys. J., Suppl. Ser., 26, 19-36 (1973)
	An optical atlas of galactic supernova remnants.
Ref:	=1978ApJS...38..119V
by	VAN DEN BERGH S.
	Astrophys. J., Suppl. Ser., 38, 119-128 (1978)
	A systematic search for galactic Supernova Remnants.
o	Fig.8: <PN VBe N> (No. 1). Table 1: <CTB NNNa> (Nos 37a, 37b).
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1974A&AS...16...71B
by	BERTAUD C. , FLOQUET M.
	Astron. Astrophys., Suppl. Ser., 16, 71-153 (1974)
	Nouveau catalogue des etoiles A a spectre particulier Ap et a raies metalliques Am.
=E=	Catalogue in electronic form as III/46
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1976MNRAS.174..267C
by	CLARK D.H. , CASWELL J.L.
	Mon. Not. R. Astron. Soc., 174, 267-305 (1976)
	A study of galactic supernova remnants, based on Molonglo-Parkes observational data.
=E=	Catalogue in electronic form as <VII/14/>
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Auth.:	DE VAUCOULEURS G.+
=E=	Catalogue in electronic form as VII/112
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Note:	1977, INSPEC Bibliography Ser. No. 2. IEE, Great Britain, Astronomical Catalogues 1951-1975.
Auth.:	COLLINS M.
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Auth.:	HODGE P.W.+
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1977A&AS...29..259M
by	MERMILLIOD J.-C. , NICOLET B.
	Astron. Astrophys., Suppl. Ser., 29, 259-261 (1977)
	A general catalogue of UBV photoelectric photometry.
o	magnetic tape
Ref:	=1983BICDS..25...79M
by	MERMILLIOD J.-C.
	Bull. Inf. Centre Donnees Stellaires, 25, 79-80 (1983)
	A complete supplement to the general catalogue of UBV photoelectric photometry.
o	Comprehensive supplement to 1977A&AS...29..259M
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1978MNRAS.182..687C
by	CALVET N. , COHEN M.
	Mon. Not. R. Astron. Soc., 182, 687-704 (1978)
	Studies of bipolar nebulae. V. The general phenomenon.
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1978A&AS...31..243R
by	ROUSSEAU J. , MARTIN N., PREVOT L., REBEIROT E., ROBIN A., BRUNET J.P.
	Astron. Astrophys., Suppl. Ser., 31, 243-None (1978)
	Studies of the Large Magellanic Cloud stellar content. III. Spectral types and V magnitudes of 1822 members.
=E=	Catalogue in electronic form as III/147
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1978POBeo...7...69S
by	SEVARLIC B.M. , TELEKI G., SZARDECZKY-KARDOSS G.
	Publ. Obs. Astron. Beograd, 7, 69-272 (1978)
	Bibliography of the Catalogues of Star Positions.
o	2087 catalogues recensed.
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1979A&AS...36..337E
by	ENGELS D.
	Astron. Astrophys., Suppl. Ser., 36, 337-345 (1979)
	Catalogue of late-type stars with OH, H2O or SiO maser emission.
=E=	Catalogue in electronic form as V/18
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1979AuJPh..32...83M
by	MILNE D.K.
	Australian J. Phys., 32, 83-92 (1979)
	A new catalogue of galactic SNRs corrected for distance from the galactic plane.
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1980DI)
by	DIXON R.S.
	Columbus Ohio Univ. Press, pp. 835 (also on magnetic tape)
	A Master List of non stellar optical astronomical objects
o	Compiled by Dixon R.S. and Sonneborn G. Overlay maps in ref. 1981DG
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1980A&A....90..269W
by	WEILER K.W. , PANAGIA N.
	Astron. Astrophys., 90, 269-282 (1980)
	Vela X and the evolution of plerions.
o	Table 3 lists 13 probable, possible or doubtful plerions.
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1981DG)
by	DIXON R.S. , GEARHART M.R., SCHMIDTKE P.C.
	Ohio State Univ. Radio Observatory
	Atlas of sky overlay maps
o	1037 overays SAO stars, all catalogued non-stellar objects in ref. 1980DI ; coordinates grids (α , δ 1950, galactic coordinates and ecliptic)
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1981A&AS...45..207R
by	RUFENER F.
	Astron. Astrophys., Suppl. Ser., 45, 207-366 (1981)
	Third catalogue of stars measured in the Geneva Observatory photometric system.
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Auth.:	SANDAGE A.+
=E=	Catalogue in electronic form as VII/51
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1982FM)
by	FERNANDEZ A. , MATHEZ G., MAZURE A., NOTTALE L., ROTHENFLUG R.
	IAU Coll. 64, Strasbourg 1981 "Automated Data Retrieval in Astronomy", C. Jaschek and W. Heintz, eds, Reidel, Dordrecht, p. 265-271
	Le Centre de Donnees des Amas de Galaxies (CEDAG)
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1982GS A)
by	GEZARI D.Y. , SCHMITZ M., MEAD J.M.
	NASA TM 83-819
	Catalogue of Infrared Observations
o	about 56000 individual observations of about 10000 infrared sources ordering by α (1950) Alphabetical index of names: part V (orange pages) Superseded by 1984GS
+Ref:	(#1982GS B), GEZARI D.Y., SCHMITZ M., MEAD J.M.
	NASA TM 84-001
	Far infrared supplement: Catalog of Infrared Observations
o	Selection of sources emitting at λ≥5 µm among 1982GS Superseded by 1984GS
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1982POBeo..29...71S
by	SEVARLIC B.M. , TELEKI G., KNEZEVIC Z.
	Publ. Obs. Astron. Beograd, 29, 71-97 (1982)
	Bibliography of the photographic catalogues of star positions.
o	140 catalogues from years 1955 to 1975
Ref:	=1982POBeo..29...99S
by	SEVARLIC B.M. , TELEKI G., KNEZEVIC Z.
	Publ. Obs. Astron. Beograd, 29, 99-124 (1982)
	Bibliography of Stellar Atlases, Maps and Charts.
o	261 entries from years 1537 to 1973.
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1982A&AS...48..383V
by	VOGT N. , BATESON F.M.
	Astron. Astrophys., Suppl. Ser., 48, 383-407 (1982)
	An atlas of southern and equatorial dwarf novae.
Ref:	=1992A&AS...93..463B
by	BRUCH A. , MEIJER J., NAUMANN M., SCHIMPKE T., UNGRUHE R., VOGT N.
	Astron. Astrophys., Suppl. Ser., 93, 463-468 (1992)
	An astrometric catalogue of southern and equatorial dwarf novae.
=E=	Catalogue in electronic form as J/A+AS/93/463
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1983BICDS..24..125D
by	DUBOIS P. , OCHSENBEIN F., PATUREL G.
	Bull. Inf. Centre Donnees Stellaires, 24, 125-None (1983)
	Extension of SIMBAD toward galaxies.
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1983MO)
by	MOREL M.
	Published by M. Morel, 18 Elizabeth Cook Drive, Rankin Park NSW 2287, Australia
	A Visual Atlas of the Large Magellanic Cloud
o	Atlas for observers with telescope of moderate aperture. 5 tables ; 7 charts ; 1950 coordinates Contents include these objects : -277 of some of the brightest variable stars (HV and NSV) -nonstellar objects from NGC, IC and other lists entries in several lists of LMC members -hundreds of stars with known V magnitude
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1984PASAu...5..369A
by	ALLEN D.A.
	Proc. Astron. Soc. Australia, 5, 369-421 (1984)
	A catalogue of symbiotic stars.
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1984A&AS...55..371C
by	CATALANO F.A. , RENSON P.
	Astron. Astrophys., Suppl. Ser., 55, 371-392 (1984)
	Catalogue des periodes observees pour des etoiles Ap.
Ref:	=1988A&AS...72....1C
by	CATALANO F.A. , RENSON P.
	Astron. Astrophys., Suppl. Ser., 72, 1-7 (1988)
	Premier supplement au catalogue des periodes observees pour des etoiles Ap.
Ref:	=1991A&AS...87...59C
by	CATALANO F.A. , RENSON P., LEONE F.
	Astron. Astrophys., Suppl. Ser., 87, 59-68 (1991)
	Second supplement to the catalogue of observed periods of Ap stars.
Ref:	=1993A&AS...98..269C
by	CATALANO F.A. , RENSON P., LEONE F.
	Astron. Astrophys., Suppl. Ser., 98, 269-273 (1993)
	Third supplement to the catalogue of observed periods of Ap stars.
=E=	Catalogue in electronic form as III/152
=E=	Catalogue in electronic form as III/199
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1984GS A)
by	GEZARI D.Y. , SCHMITZ M., MEAD J.M.
	NASA RP-1118, 1st edition (May 1984)
	Catalog of Infrared Observations
o	Updates and supersedes 1982GS Scientific journals searched for the complete period 1965-1982 Over 85000 individual observations of about 10000 different infrared sources.
+Ref:	(#1984GS B), SCHMITZ M., MEAD J.M., GEZARI D.Y.
	NASA RP-1182
	Infrared Source Cross-Index, First edition
o	A compilation, not a critical analysis of published positions
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1984ApJS...56..403K
by	KOWALSKI M.P. , ULMER M.P., CRUDDACE R.G., WOOD K.S.
	Astrophys. J., Suppl. Ser., 56, 403-506 (1984)
	An X-ray survey of clusters of galaxies. IV. A survey of southern clusters and a compilation of upper limits for both Abell and southern clusters.
=E=	Catalogue in electronic form as J/ApJS/56/403
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1984BICDS..27..141M
by	MERMILLIOD J.C.
	Bull. Inf. Centre Donnees Stellaires, 27, 141-143 (1984)
	Preliminary catalogue of photographic UBV photometry for stars in open clusters.
o	34000 stars in 127 open clusters.
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1984A&AS...57..385R
by	RITTER H.
	Astron. Astrophys., Suppl. Ser., 57, 385-418 (1984)
	Catalogue of cataclysmic binaries, low-mass X-ray binaries and related objects. (Third edition).
Ref:	=1987A&AS...70..335R
by	RITTER H.
	Astron. Astrophys., Suppl. Ser., 70, 335-367 (1987)
	Catalogue of cataclysmic binaries, low-mass X-ray binaries and related objects (fourth edition).
Ref:	=1990A&AS...85.1179R
by	RITTER H.
	Astron. Astrophys., Suppl. Ser., 85, 1179-1256 (1990)
	Catalogue of cataclysmic binaries, low-mass X-ray binaries and related objects (fifth edition).
=E=	Catalogue in electronic form as V/37
=E=	Catalogue in electronic form as V/59
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1985A&AS...60...61H
by	HAUCK B. , MERMILLIOD M.
	Astron. Astrophys., Suppl. Ser., 60, 61-62 (1985)
	uvby-β photoelectric photometric catalogue (magnetic tape).
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1986A&AS...65...59B
by	BARBIER-BROSSAT M. , PETIT M.
	Astron. Astrophys., Suppl. Ser., 65, 59-61 (1986)
	Catalogue bibliographique de vitesses radiales stellaires.
Ref:	=1990A&AS...85..885B
by	BARBIER-BROSSAT M. , PETIT M., FIGON P., GERBAL M., MARTIN S.
	Astron. Astrophys., Suppl. Ser., 85, 885-888 (1990)
	Catalogue bibliographique de vitesses radiales stellaires.
=E=	Catalogue in electronic form as III/160
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1986JRASC..80...51H
by	HIGGS L.A.
	J. R. Astron. Soc. Can., 80, 51-54 (1986)
	The designation of radio sources observed with the DRAO synthesis telescope.
o	No objects. Retroctive designation for Penticton sources lists 1P, 2P, 3P, 4P, 5P
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1987A&AS...70..481B
by	BRUCH A. , FISCHER F.J., WILMSEN U.
	Astron. Astrophys., Suppl. Ser., 70, 481-516 (1987)
	An atlas and catalogue of northern dwarf novae.
o	(Erratum) erratum vol 74, 351 for TZ Per.
=E=	Catalogue in electronic form as J/A+AS/70/481
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1987GS A)
by	GEZARI D.Y. , SCHMITZ M., MEAD J.M.
	NASA RP-1196
	Catalog of Infrared Observations
o	2nd Edition (1st edition is ref. 1984GS) Updated by 1993GS
o	Part I. Data (λ1 to 1000 µm) Part II. Appendices A: Index of IR source positions B: Bibliography ordered chronologically C: First author alphabetical order listing D: Spectrum atlas Compilation in original published form with no attempt to create a single system of infrared photometric units.
+Ref:	(#1987GS B), GEZARI D.Y., SCHMITZ M., MEAD J.M.
	NASA RP-1205
	Far Infrared Supplement: Catalog of Infrared Observations
o	Subset of the data of ref. 1987GS A (NASA RP 1196) restricted to observations at λ≥5 µm
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1988HE)
by	HECK A.
	Special Publ. of the CDS, No. 11 (also magnetic tape)
	A Bibliographical catalogue of RR Lyr stars
o	6357 RR Lyr, cross-identif., bibliographical catalogue. Updates Heck and Lakaye, 1977, Astr. Astrophys. Suppl. 30, 397
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1988BICDS..35..145L
by	LORTET M.C.
	Bull. Inf. Centre Donnees Stellaires, 35, 145-154 (1988)
	A provisory catalogue of S-Dor candidate stars in the Magellanic Clouds.
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1988BICDS..34..107R
by	RENSON P.
	Bull. Inf. Centre Donnees Stellaires, 34, 107-115 (1988)
	Erreurs de designations d'etoiles Ap ou Am.
o	Erroneous designations which appeared in the literature for Ap and Am stars.
Ref:	=1988A&AS...76..127R
by	RENSON P.
	Astron. Astrophys., Suppl. Ser., 76, 127-135 (1988)
	Liste des etoiles Ap et Am dans des amas ouverts.
o	(Erratum) + erratum vol 78, 533
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1989A&AS...80...67B
by	BARBIER-BROSSAT M.
	Astron. Astrophys., Suppl. Ser., 80, 67-71 (1989)
	Catalogue de vitesses radiales moyennes stellaires (catalogue sur bande magnetique).
=E=	Catalogue in electronic form as III/161
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1989A&AS...81..323E
by	ENGELS D. , HESKE A.
	Astron. Astrophys., Suppl. Ser., 81, 323-334 (1989)
	A reference catalogue of maser and thermal emission from circumstellar SiO molecules.
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1989A&AS...81..401M
by	MERMILLIOD J.-C. , NITSCHELM C.
	Astron. Astrophys., Suppl. Ser., 81, 401-407 (1989)
	Up-to-date DDO photoelectric photometric catalogue.
o	Objects in the catalogue are not in SIMBAD
=E=	Catalogue in electronic form as II/164
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1989MO)
by	MOREL M.
	Published by M. Morel, 18 Elizabeth Cook Drive, Rankin Park NSW 2287, Australia
	A Visual Atlas of the Small Magellanic Cloud
o	This Atlas consists of the following parts: -Catalogues of plotted objects (clusters and nebulae; variable stars) presented as appendices -Master charts A and B covering the entire SMC region 0h15m < alpha < 1h45m, -76°< δ< -70° -Stars down to V = 14.0 or 14.5 -Ten large scale charts showing certain interesting areas of the SMC in greater detail and resolution Appendix 1 : clusters and nebulae Appendix 2 : variables stars Appendix 3 : index to HV stars Appendix 4 : suspected variables Appendix 5 : precession tables Charts for selected areas
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	=1989A&AS...78..469R
by	RUFENER F.
	Astron. Astrophys., Suppl. Ser., 78, 469-481 (1989)
	Catalogue of stars measured in the Geneva Observatory photometric system (fourth edition).
o	Updates 1981A&AS...45..207R.
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1990BL) =1990ApJS...74..911B
by	BENSON P.J. , LITTLE-MARENIN I.R., WOODS T.C., ATTRIDGE J.M., BLAIS K.A., RUDOLPH D.B., RUBIERA M.E., KEEFE H.L.
	Ap.J.Suppl. 74, 911-1074
	A catalog of observations for stellar masers
o	Catalog of almost 3000 stellar sources which have been searched for maser emission from the H2O, SiO, and/or OH molecules Of the sources listed, 368 were detected in H2O, 209 in SiO, and 713 in OH.
o	Table 1 : (Nos 1-2958) ; 1950 coordinates ; alternate names (many IRAS names are not quoted, the IRAS PSC was not searched) the galactic coordinates are not quoted (p. 913-960) Table 2 : References for both detections and nondetections (N means not detected) for each of the three molecules (p. 961-1060) Table 3 : References ordered by code order (p. 1061-1069)
=E=	Catalogue in electronic form as V/68
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1990NM A) =1990A&AS...82..331N
by	NITSCHELM C. , MERMILLIOD J.C.
	Astr. Astrophys. Suppl. 82, 331-337
	Up-to-date Walraven VBLUW photoelectric photometric catalogue
o	The up-to-date catalogue, on magnetic tape, contains the data published until the end of 1988 (6022 measurements, for 5564 stars) The stars are identified by their Lausanne Identif. code (LID) ; numerous cross-identif. ; 1950 coordinates Updates Python, 1979 Astr. Astrophys. Suppl. 38, 463-464
+Ref:	(#1990NM B) =1990A&AS...85..839N
by	NITSCHELM C. , MERMILLIOD J.C.
	Astr. Astrophys. Suppl. 85, 839-844
	Photometric catalogue in the Eggen modified uvby system
o	The catalogue, on magnetic tape, contains the data published until the end of 1989 (5036 measurements, for 4469 stars) The stars are identified by their Lausanne Identif. code (LID) ; numerous cross-identif. ; 1950 coordinates
=E=	Catalogue in electronic form as II/163
=E=	Catalogue in electronic form as II/165
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1990SI)
by	SCHWERING P.B.W. , ISRAEL F.P.
	Kluwer Academic Publ., 224pp.
	Atlas and catalogue of infrared sources in the Magellanic Clouds
o	Contents: 1. Introduction 2. Infrared source identification tables (correlation with several optical catalogues) 3. The Leiden-IRAS Magellanic Clouds Infrared source catalogues 4. Atlas of infrared emission of the Magellanic Clouds Maps based on observations obtained in the Additional Observations (AO) program, in the Deep Sky Mapping (DPM) mode Overall maps: SMC p. 104-105 4.3° x 4.3° LMC p. 126-127 8.5° x 8.5° Detail maps: SMC p. 106-125 2.1° x 2.1° LMC p. 128-205 2.1° x 2.1° Parts 2 and 3 are included in 1989A&AS...79...79S (SMC) and 1989A&AS...79..105S (LMC), acronyms LI-SMC and LI-LMC
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1990WH) =1990A&AS...86..357W
by	WALTER H.G. , HERING R., DE VEGT Ch.
	Astr. Astrophys. Suppl. 86, 357-393
	An astrometric catalogue of radio sources
o	Available both as a printed version and an updated magnetic tape
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1991DV A)
by	DE VAUCOULEURS G. , DE VAUCOULEURS A., CORWIN H.G.Jr, BUTA R.J., PATUREL G., FOUQUE P.
	Springer-Verlag
	Third Reference Catalogue of Bright Galaxies
o	1st Vol., explanations, references, cross-identif. tables. 2nd and 3rd Vol. are the Catalogue proper, often quoted as the RC3 catalogue. N = 23024 objects
+Ref:	(#1991DV B) =1994AJ....108.2128C
by	CORWIN H.G.Jr , BUTA R.J., DE VAUCOULEURS G.
	A.J. 108, 2128-2144
	Corrections and additions to the Third Reference Catalogue of Bright Galaxies
=E=	Catalogue in electronic form as VII/155
=E=	Catalogue in electronic form as J/AJ/108/2128
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1991P3) =1991A&AS...90....1P
by	PERIE J. , PREVOT L., ROUSSEAU M., PEYRIN Y., ROBIN A.
	Astr. Astrophys. Suppl. 90, 1-17
	Positional reference stars in the Magellanic Clouds
o	Equatorial coordinates determined for 926 stars (mainly foreground to the Magellanic Clouds) Accuracy characterized by mean values O-C 0.35" and 0.38", from the coordinates of the Perth reference stars. Table 1 : members of LMC and SMC, measured in the catalogue. Table 2 : catalogue ; 2000 coordinates ; CPD number cross-identif. (when available) with HD, CPC, SAO, Perth. Don't use the internal number given in col. 1. Identif. charts for 35 double or multiple stars.
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1991RE) =1991ESOSR..11....1R
by	REIPURTH B. , BRAND J., WOUTERLOOT J.G.A., HERBIG G.H., PETTERSSON B., SCHWARTZ R.D., NYMAN L.-A., KRAUTTER J., GRAHAM J.A., WILKING B.A., EIROA C.
	ESO Scientific Report No. 11, pp. 211, ed. B. Reipurth
	Low Mass Star Formation in Southern Molecular Clouds
o	Contents: Low Mass Star Formation in Orion p. 1 Brand J., Wouterlout J.G.A. The Canis Majoris OB1 Association p. 59 Herbig G.H. Low Mass Star Formation in Puppis and Vela p. 69 Pettersson B. The Chamaleon Dark Clouds and T-Associations p. 93 Schwartz R.D. The Southern Coalsack - Where are all the Young Stars? p. 119 Nyman L.-A. The Star Forming Region in Lupus p. 127 Krautter J. Young Low Mass Stars in the Norma Cloud p. 149 Reipurth B., Graham J.A. Star Formation in the Ophiuchus Molecular Cloud Complex p. 159 Wilking B.A. Star Formation in the Corona Australis Region p. 185 Graham J.A. The Serpens Molecular Cloud p. 197 Eiroa C.
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1991RG A) =1991A&AS...89..429R
by	RENSON P. , GERBALDI M., CATALANO F.A.
	Astron. Astrophys., Suppl. Ser., 89, 429-434 (1991)
	General catalogue of Ap and Am stars.
o	catalog: <Renson NNNNN> N=6684 among (Nos 10-61970).
+Ref:	(#1991RG B) =1991A&AS...89...61R
by	RENSON P. , KOBI D., NORTH P.
	Astr. Astrophys. Suppl. 89, 61-76
	A database of Ap stars
o	The database can be used on an IBM-compatible personal computer. It is essentially based on Renson's general catalogue (ref. 1991RG). N = 3195 Ap stars
=E=	Catalogue in electronic form as III/162
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1992GS) =1992ApJS...81..795G
by	GRILLO F. , SCIORTINO S., MICELA G., VAIANA G.S., HARNDEN F.R.Jr
	Ap.J.Suppl. 81, 795-863
	An Einstein Observatory SAO-based catalog of B-type stars
o	Emission between 0.16 and 4.0 keV (IPC images) from 1545 B-type SAO stars Table 1 : Optical data Table 2 : X-ray data
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1992HA) =1992BICDS..40...19H
by	HAUCK B.
	Bull. Inf. CDS 40, 19-21
	Fourth catalogue of Am stars with known spectral types
o	2890 determinations for 2152 stars. Obsoletes Hauck 1986, Astr. Astrophys. Suppl. 64, 21
Details on Acronym: (compilation, no acronym)
(compilation, no acronym)
Ref:	(#1993GS A)
by	GEZARI D.Y. , SCHMITZ M., PITTS P.S., MEAD J.M.
	NASA RP-1294
	Catalog of Infrared Observations
o	3rd Edition. Updates 1987GS A and B (2nd edition) Produced as a single volume. Complete for 1965 through 1990 ; 206000 individual observations. The catalog data are presented as published in the original articles. Contents: Introduction (with source name abbreviations and references) Catatalogue of Infrared observations Appendix A: Atlas of Infrared spectral ranges Appendix B: Bibliography of infrared astronomy (alphabetical order) Appendix C: Bibliography of infrared astronomy (chronological order) Appendix D: Index of infrared source positions (alphabetical order)
+Ref:	(#1993GS B), GEZARI D.Y., SCHMITZ M., PITTS P.S., MEAD J.M.
	NASA RP-1295
	Far Infrared Supplement: Catalog of Infrared Observations
=E=	Catalogue in electronic form as II/184
=E=	Catalogue in electronic form as II/216
=E=	Catalogue in electronic form as II/225
Details on Acronym: A
A	(Asiago) (Not yet in Simbad)
Write:	<<A NNNN>>
Object:	Flare * (SIMBAD class: Eruptive* = Eruptive Variable)
Rem:	V* Nomenclature.
Details on Acronym: A
A	(Ariel satellite)
*****	Avoid the usage of A, prefer 1A
Details on Acronym: A
A	(Astrographic catalog)
*****	Avoid the usage of A, prefer AC
Details on Acronym: A
A	(Abell+)
====>	Equivalent to: ACO
Details on Acronym: A
A	(Aitken)
*****	Avoid the usage of A, prefer ADS
Details on Acronym: A
A	(Arecibo general catalog)
*****	Avoid the usage of A, prefer AGC
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: A
A	(Andrews)
*****	Avoid the usage of A, prefer Andrews
Origin	of the Acronym: L = Found in the literature
Details on Acronym: A
A	(Anonymous)
*****	Avoid the usage of A, prefer Anon
Details on Acronym: A
A	(Arp)
*****	Avoid the usage of A, prefer APG
Details on Acronym: A
A	(Ardeberg+)
*****	Avoid the usage of A, prefer Ardb
Origin	of the Acronym: L = Found in the literature
Details on Acronym: A
A	(Abell)
*****	Avoid the usage of A, prefer Palomar
Details on Acronym: A
A	(cloud complex labelled A)
*****	Avoid the usage of A, prefer [GVC73]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: A
A	(cloud complex labelled A)
Note:	HVC Complex A
*****	Avoid the usage of A, prefer [H68]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: A
A	(Abell)
*****	Avoid the usage of A, prefer A55
Details on Acronym: A
A	(Abell, 1966)
*****	Avoid the usage of A, prefer A66
Details on Acronym: A
A	(ASCA observation)
*****	Avoid the usage of A, prefer [YHK98]
Origin	of the Acronym: L (2000A&A...355..629A)
Details on Acronym: A'
A'	(Abell)
*****	Avoid the usage of A', prefer A66
Details on Acronym: A-F
A-F	(A-F type *)
*****	Avoid the usage of A-F, prefer Case A-F
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: A.D.
A.D.	(Anno Domini)
*****	Avoid the usage of A.D., prefer SN
Details on Acronym: 1A
1A	(Ariel satellite, list 1)= (A) = (Ariel)
Write:	<<1A HHMM+DD>> <<1A HHMM+DDd>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Details on Acronym: A1
A1	(Asiago obs., field 1)
Write:	<<A1 NNN>>
N:	129
Object:	Blue Obj. (SIMBAD class: blue = Blue Object)
Stat:	is completely incorporated in Simbad
Note:	field centered l= 243deg, b = 67deg Identif. charts ref. 1982A&AS...48..333E gives the physical nature of the A1 objects.
Ref:	=1968POPad.143....1B
by	BARBIERI C. , ERCULIANI L., ROSINO L.
	Publ. Oss. Astron. Padova, 143, 1-14 (1968)
	Studies of blue objects in high galactic latitudes. I. Blue faint objects in the field of 88 Leonis.
o	<A1 NNN> (Nos 1-129)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 2A
2A	(Ariel satellite, list 2)= (Ariel)
Write:	<<2A HHMM+DD>> <<2A HHMM+DDd>>
N:	105
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Group: Leicester. Error box: 01 to 0.5 sq.deg
Ref:	=1978MNRAS.182..489C
by	COOKE B.A. , RICKETTS M.J., MACCACARO T., PYE J.P., ELVIS M., WATSON M.G., GRIFFITHS R.E., POUNDS K.A., McHARDY I., MACCAGNI D., SEWARD F.D., PAGE C.G., TURNER M.J.L.
	Mon. Not. R. Astron. Soc., 182, 489-515 (1978)
	The Ariel V SSI catalogue of high galactic latitude (\|b\|>10) X-ray sources.
o	<2A HHMM+DDd> N=105
=E=	Catalogue in electronic form as VII/19
Details on Acronym: A2
A2	(Asiago obs., field 2)
Write:	<<A2 NNN>>
N:	487
Object:	Blue Obj. (SIMBAD class: blue = Blue Object)
Ref:	=1972Ap&SS..16..324B
by	BARBIERI C. , ROSINO L.
	Astrophys. Space Sci., 16, 324-335 (1972)
	Studies of blue objects at high galactic latitudes. Faint blue objects in the field of BD +29 2348 (the Galactic North Pole).
o	Table I: <A2 NNN> Nos among (Nos 1-487)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [A2001]
[A2001]	(Arp, 2001)
Write:	<<[A2001] Mrk 273 NN>> <<[A2001] Mrk 273 NNW>> <<[A2001] Mrk 231 NNN.N>> <<[A2001] Mrk NNN NNN>> <<[A2001] Arp 220 NN>> <<[A2001] Arp 220 NN.N>> <<[A2001] Arp 220 NN.NW>> <<[A2001] NGC 6240 NN>> <<[A2001] NGC 383 A>>
N:	13+14+10+11+14+10
Object:	(X) + G (SIMBAD class: X = X-ray Source)
Note:	Fig.7, Table 1: bright X-ray sources in the field of Mrk 273. Fig.12, Table 2: bright X-ray sources in the field of Mrk 231. The format 'NNN.N' stands for counts kpc(-1). Fig.17: standard detection of X-ray sources in the field APG 220. Fig.18, Table 3: bright X-ray sources in the field of APG 220. The format 'NN.NW' stands for counts ks(-1). Fig.21: ROSAT PSPC sources around NGC 6240. Fig.25: N=10 galaxies in group SW of NGC 383.
Ref:	=2001ApJ...549..780A
by	ARP H.
	Astrophys. J., 549, 780-801 (2001)
	The surroundings of disturbed, active galaxies.
o	Figs 19, 22, 27: Objects without designation are not in SIMBAD.
o	Fig.7, Table 1: <[A2001] Mrk 273 NNW> N=13. Fig.12, Table 2: <[A2001] Mrk 231 NNN.N> N=14. Fig.17: <[A2001] Arp 220 NN> (Nos 1-10). Fig.18, Table 3: <[A2001] Arp 220 NN.NW> N=11. Fig.21: <[A2001] NGC 6240 NN> (Nos 1-14). Fig.25: <[A2001] NGC 383 A> (Nos A-J).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A2006]
[A2006]	(Antipin, 2006)
Write:	<<[A2006] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of SN 1985U.
Ref:	=2006IAUC.8665....2A
by	ANTIPIN S.V.
	IAU Circ., 8665, 2-None (2006)
	Supernova 1985U.
o	<[A2006] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A2017]
[A2017]	(Agnello, 2017)
Write:	<<[A2017] WGN>>
N:	4
Object:	Poss. Stream (SIMBAD class: Stream = Stellar Stream)
Stat:	is completely incorporated in Simbad
Note:	N=4 Galactic stream candidates. Use of WISE and Gaia DR1 data.
Ref:	=2017MNRAS.471.2013A
by	AGNELLO A.
	Mon. Not. R. Astron. Soc., 471, 2013-2021 (2017)
	Quasar lenses and galactic streams: outlier selection and Gaia multiplet detection.
o	Paragr. 3.3: <[A2017] WGN> (Nos WG1-WG4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A2018]
[A2018]	(Araya, 2018)= ([A2018a])
Write:	<<[A2018] G350.6-04.7>>
N:	1
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	N=1 extended gamma-ray source, discovered in Fermi LAT data.
Ref:	=2018MNRAS.474..102A
by	ARAYA M.
	Mon. Not. R. Astron. Soc., 474, 102-107 (2018)
	Discovery of an extended source of γ-ray emission in the Southern hemisphere.
o	<[A2018] G350.6-04.7> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A2018a]
[A2018a]	(Araya, 2018)
*****	Avoid the usage of [A2018a], prefer [A2018]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A2018b]
[A2018b]	(Agnello, 2018)
Write:	<<[A2018b] WG J0214-2105>> <<[A2018b] WG J021416.37-210535.3>> <<[A2018b] WG J0214-2105 A>> <<[A2018b] WG J0214-2105 lens>> <<[A2018b] WG021416.37-210535.3>> (not recognised by Simbad, but found in literature) <<[A2018b] WG0214-2105>>
N:	1+1+4+1
Object:	Grav. lens system + QSO + Grav. lensed image of a QSO + Grav. lens (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=1 gravitational lens system, N=4 gravitationally lensed images of N=1 QSO, and N=1 gravitational lens, from WISE and Gaia-DR2 data.
Ref:	=2018RNAAS...2b..42A
by	AGNELLO A.
	RNAAS, 2b, 42 (2018)
	WG021416.37-210535.3, a quadruply lensed quasar in three public surveys.
o	<[A2018b] WG J0214-2105> N=1, <[A2018b] WG J021416.37-210535.3> N=1, <[A2018b] WG J0214-2105 A> (Nos A-D), <[A2018b] WG J0214-2105 lens> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A2018c]
[A2018c]	(Champagne+Decarli+Casey+, 2018)
Write:	<<[A2018c] NN>>
N:	10
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra HRC-I observations of N=10 X-ray sources in the field of Alpha Centauri.
Ref:	=2018AJ....156..274A
by	AYRES T.R.
	Astron. J., 156, 274-274 (2018)
	Serendipitous X-ray sources in the Chandra HRC field around Alpha Centauri.
o	Fig. 1, Table 2: <[A2018c] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 3A
3A	(Ariel satellite, list 3)= (Ariel)
Write:	<<3A HHMM+DDd>>
N:	251
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Ref:	=1981MNRAS.197..893M
by	McHARDY I.M. , LAWRENCE A., PYE J.P., POUNDS K.A.
	Mon. Not. R. Astron. Soc., 197, 893-919 (1981)
	The Ariel V (3A) catalogue of X-ray sources. II. Sources at high galactic latitude (\|b\| > 10 °).
o	Table 1: <3A HHMM+DDd> N=142
Ref:	=1981MNRAS.197..865W
by	WARWICK R.S. , MARSHALL N., FRASER G.W., WATSON M.G., LAWRENCE A., PAGE C.G., POUNDS K.A., RICKETTS M.J., SIMS M.R., SMITH A.
	Mon. Not. R. Astron. Soc., 197, 865-891 (1981)
	The Ariel V (3A) catalogue of X-ray sources. I. Sources at low galactic latitude (\|b\|<10 °.).
o	Table 2: <3A HHMM+DDd> N=109
Details on Acronym: A3
A3	(Asiago obs., field 3)= (BB)
Write:	<<A3 NNN>>
N:	506
Object:	Blue Obj. (SIMBAD class: blue = Blue Object)
Ref:	=1974A&AS...13..269B
by	BARBIERI C. , BENVENUTI P.
	Astron. Astrophys., Suppl. Ser., 13, 269-291 (1974)
	Studies of blue objects at high galactic latitudes. III. Faint blue objects in the field of BD +15 2469.
o	<A3 NNN> N=324 among (Nos 1-506)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: A55
A55	(Abell, 1955)= (A) = (Abel) = (Abell)
Write:	<<PN A55 NN>>
N:	73
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Obsolete, PK Nomenclature.
Ref:	=1955PASP...67..258A
by	ABELL G.O.
	Publ. Astron. Soc. Pac., 67, 258-261 (1955)
	Globular clusters and planetary nebulae discovered on the national geographic society-Palomar Observatory sky survey.
o	Table I: <Cl Palomar NN> (Nos 1-13), Table II: <PN A55 NN> (Nos 1-73)
Details on Acronym: [A56]
[A56]	(Arp, 1956)
Write:	<<[A56] NN>>
N:	30
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Note:	Table 1, Plate
in source:	M 31 = NGC 224
Ref:	=1956AJ.....61...15A
by	ARP H.C.
	Astron. J., 61, 15-34 (1956)
	Novae in the Andromeda nebula.
o	T.II: photoelectric stds not in Simbad
o	T.I: <[A56] NN> N=30
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A58]
[A58]	(Arp, 1958)
Write:	<<[A58] A>> <<[A58] a>>
N:	37
Object:	* (SIMBAD class: Star)
Note:	Table V: (Nos A-Z) and (a-k). Nos j and k are added in 1960AJ.....65..404A
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1958AJ.....63..118A
by	ARP H.C.
	Astron. J., 63, 118-127 (1958)
	Southern hemisphere photometry. II. Photoelectric measures of bright stars.
o	Table V: <[A58] A> (Nos A-Z), <[A58] a> (Nos a-i), Table VI: <Cl* NGC 1866 ARP A> (Nos A-I), Table VII: <Cl* NGC 5139 ARP A> (Nos A-K)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A61]
[A61]	(Abell, 1961)= (Abell)
Write:	<<[A61] NN>>
N:	17
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Ref:	=1961AJ.....66..607A
by	ABELL G.O.
	Astron. J., 66, 607-613 (1961)
	Evidence regarding second-order clustering of galaxies and interactions between clusters of galaxies.
o	Table II: <[A61] NN> (Nos 1-17)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A63]
[A63]	(Argue, 1963)= (Argue)
Write:	<<[A63] NN NNN>>
N:	128
Object:	* (SIMBAD class: Star)
Note:	KPNO photometric observations of the Coma region.
Ref:	=1963MNRAS.127...97A
by	ARGUE A.N.
	Mon. Not. R. Astron. Soc., 127, 97-104 (1963)
	Photographic photometry with the Cambridge Schmidt telescope. II. Photoelectric UBV calibrations in the Coma region.
o	Table I: <[A63] NN NNN> N=128.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A64]
[A64]	(Apriamashvili, 1964)
Write:	<<[A64] Red +DD NNNa>>
N:	490+407
Object:	* (SIMBAD class: Star)
Note:	N=490+407 red stars in the Aquila and Scutum regions.
in source:	NAME Aql Region
in source:	NAME Scutum Region
Ref:	=1964AbaOB..31...27A
by	APRIAMASHVILI S.P.
	AbaOB, 31, None (1964)
	The catalogue of photographic magnitudes, color-indices, spectra and luminosities of faint stars in two regions of the milky way in Aquila and Scutum.
o	<[A64] Red +DD NNNa> N=490+407.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: A66
A66	(Abell, 1966)= (A) = (A') = (Abell)
Write:	<<PN A66 NN>>
N:	86
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	A few objects have Identif. charts
Ref:	=1966ApJ...144..259A
by	ABELL G.O.
	Astrophys. J., 144, 259-279 (1966)
	Properties of some old planetary nebulae.
o	Table 2: <PN A66 NN> (Nos 1-86)
Details on Acronym: [A66]
[A66]	(Artiukhina, 1966)
Write:	<<[A66] R NNN>> <<[A66] Art R.NNN>> (not recognised by Simbad, but found in literature)
Object:	* (SIMBAD class: Star)
Note:	Stars in the field of the open cluster NGC 2632.
in source:	NGC 2632 = NAME PRAESEPE
Ref:	=1966TrSht..35..111A
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A68]
[A68]	(Andrews)
Write:	<<[A68] a>>
N:	3
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=3 comparison stars to YZ CMi.
Ref:	=1968IBVS..265....1A
by	ANDREWS A.D.
	IAU Inform. Bull. Var. Stars, 265, 1-4 (1968)
	Flares and mean photometry of YZ Canis Minoris.
o	Table 2: <[A68] a> (Nos a-c).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A69]
[A69]	(Albers, 1969) (Not yet in Simbad)
Write:	<<[A69] NN>>
N:	76
Object:	Supergiant * (SIMBAD class: Star)
Note:	See also paper II: [A72c].
Ref:	=1969ApJ...156L..37A
by	ALBERS H.
	Astrophys. J., 156, 37-40 (1969)
	Infrared surveys of the Southern Milky Way. I. Suspected supergiant stars.
o	Table 1: <[A69] NN> (Nos 1-76).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A70]
[A70]	(Ackermann, 1970)
Write:	<<[A70] LL-BB-NNN>>
N:	166+86+12+134
Object:	(IR) + * (SIMBAD class: Star)
Note:	Infrared stars in four fields, centered at LL, BB
Ref:	=1970A&A.....8..315A
by	ACKERMANN G.
	Astron. Astrophys., 8, 315-334 (1970)
	Extreme red stars, in Cygnus.
o	Appendix: <[A70] LL-BB-NNN> N=166+86+12+134.
=E=	Catalogue in electronic form as II/260
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A71]
[A71]	(Angione, 1971)
Write:	<<[A71] PHL NNN A>> <<[A71] HHMM+DD A>> <<[A71] HHMM+DD A'>> <<[A71] 3C NNN.N N>> <<[A71] 3C NNN.N A'>> <<[A71] 3C NNN.N A>> <<[A71] Ton NNNN A>> <<[A71] Ton NNNN A'>>
N:	167
Object:	* (SIMBAD class: Star)
Note:	N=167 stars in the field of N=25 QSO. Finding charts.
Ref:	=1971AJ.....76..412A
by	ANGIONE R.J.
	Astron. J., 76, 412-418 (1971)
	Photoelectric sequences for the brighter QSO's.
o	Table II: <[A71] PHL 658 A>, <[A71] HHMM+DD A>, <[A71] HHMM+DD A'>, <[A71] 3C NNN N>, <[A71] 3C NNN A>, <[A71] 3C NNN A'>, <[A71] 3C NNN.N N>, <[A71] 3C NNN.N A>, <[A71] Ton NNNN A>, <[A71] Ton NNNN A'>, N=167.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A72a]
[A72a]	(Allen, 1972)= (IRS)
Write:	<<[A72a] M1-82 IRS N>>
N:	3
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Mount Wilson 152cm telescope NIR observations.
in source:	PN M 1-82
Ref:	=1972ApJ...172L..55A
by	ALLEN D.A.
	Astrophys. J., 172, 55-58 (1972)
	Infrared objects in H II regions.
o	<NAME ALLEN IRS>. Table 3: <[A72a] M1-82 IRS N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A72b]
[A72b]	(Arp, 1972)= (HA) (Not yet in Simbad)
Write:	<<[A72b] N>>
N:	7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1972ApJ...174L.111A
by	ARP H.
	Astrophys. J., 174, 111-114 (1972)
	A grouping of radio sources in the area of NGC 7331 and Stephan's Quintet.
o	Table 1: <[A72b] N> (Nos 1-7)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A72c]
[A72c]	(Albers, 1972)
Write:	<<[A72c] NNN>>
N:	170
Object:	Poss. Supergiant * (SIMBAD class: Star)
Note:	See also paper I: [A69].
Ref:	=1972ApJ...176..623A
by	ALBERS H.
	Astrophys. J., 176, 623-628 (1972)
	Infrared surveys of the Southern Milky Way. II. Suspected supergiant M stars.
o	Table 1: <[A72c] NNN> (Nos 1-170).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A73]
[A73]	(Arp, 1973)
Write:	<<[A73] {A\|B\|C}NN>> <<[A73] a>> <<[A73] SN>>
N:	24+18+1+4+1
Object:	HII + * (SIMBAD class: HIIReg = HII Region)
Note:	Table 2, Fig.4: Regions HII in the Stephan's quintet, (Nos A1-A24) are low redshift regions, (Nos B1-B18) are high redshift regions, No. C1. (Nos a-d) are comparison stars. No. SN is an SN in NGC 7319 = SN 1971P
in source:	Stephan's quintet = HCG 92
Ref:	=1973ApJ...183..411A
by	ARP H.
	Astrophys. J., 183, 411-439 (1973)
	Stephan's quintet of interacting galaxies.
o	Table 2, Fig.4: <[A73] ANN> (Nos A1-A24), <[A73] BNN> (Nos B1-B18), <[A73] C1> N=1, <[A73] SN> N=1, <[A73] a> (Nos a-d).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A74]
[A74]	(Alksne, 1974) (Not yet in Simbad)
Write:	<<[A74] NN>>
N:	17
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Note:	see also BC
Ref:	=1974ISKZ....1....7A
by	ALKSNE Z.
	Issl. Solntsa Krasnykh Zvezd., 1, 7-22 (1974)
	Photographic photometry of carbon stars in the field with center on l=204.4°, b=-1.3°.
o	Table 1, col(1): <[A74] NN> (Nos 1-17). Table 1, col(2): <BC N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A76]
[A76]	(Arp, 1976)= (BSO)
Write:	<<[A76] GN>> <<[A76] BSO N>>
N:	1+1
Object:	G + Blue (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Objects near NGC 5296.
Ref:	=1976ApJ...210L..59A
by	ARP H.
	Astrophys. J., 210, 59-61 (1976)
	A quasar near a companion galaxy, NGC 5296.
o	Table 1: <[A76] G1>, <[A76] BSO 1>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A77]
[A77]	(Arp, 1977)= ([A77a]) = (BSO) = (UB)
Write:	<<[A77] NGC NNNN BSO N>> <<[A77] NGC NNNN W N>> <<[A77] NGC NNNN UB N>>
N:	9
Object:	Blue Obj. (SIMBAD class: blue = Blue Object)
Note:	In 1977, International Coll. of CNRS, No. 263, p. 377
Auth.:	ARP H.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A77a]
[A77a]	(Arp, 1977)
*****	Avoid the usage of [A77a], prefer [A77]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A77b]
[A77b]	(Arp, 197)
Write:	<<[A77b] QSO a>> <<[A77b] Ch N>> <<[A77b] GN>> <<[A77b] NEQ3>> <<[A77b] NEQ3 zN>> <<[A77b] NGC NNNN knot N>> <<[A77b] MCG +7-25-48 knot N>>
N:	2+5+2+1+2+8
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Observations of the neighborouhoods of NGC 4151. N=2 QSOs (Nos o, r). N=5 galaxies in 'chain' (Letters 'Ch' in the format) west of NGC 4151. N=2 galaxies G1 and G2, G1 is a companion of NGC 4151, G2 is embedded in a filament NW of NGC 4156. NEQ3 (nonequilibrum system number 3 found around NGC 4151 by Sulentic and Arp, 1976, first year report on NSF grant.) showing a lenticular central galaxy attached to 3 compact objects, to of which are identified by their redshifts z1 and z2. HII regions in NGC 4151, NGC 4156, and +MCG 7-25-48 are described as large knots. See also [GL2004].
in source:	NGC 4151
Ref:	=1977ApJ...218...70A
by	ARP H.
	Astrophys. J., 218, 70-85 (1977)
	Neighborhoods of galaxies. II - NGC 4151.
o	Fig.3: <[A77b] QSO a> (Nos o, r). Fig.3, Table 1: <[A77b] Ch N> (Nos 1-5), <[A77b] GN> (Nos G1, G2), <[A77b] NEQ3> N=1, <[A77b] NEQ3 zN> (Nos z1, z2). Table 3: <[A77b] NGC 4151 knot N> (Nos 1-3), <[A77b] NGC 4156 knot N> (Nos 1-2), <[A77b] MCG +7-25-48 knot N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A79]
[A79]	(Allen, 1979)= (DA)
Write:	<<[A79] N>>
N:	2
Object:	WR (SIMBAD class: WolfRayet* = Wolf-Rayet)
Stat:	is completely incorporated in Simbad
Note:	N=2 new Wolf-Rayet stars in the Galactic Center field.
Ref:	=1979Obs....99...83A
by	ALLEN D.A.
	The Observatory, 99, 83-88 (1979)
	On planetary nebulae and Wolf-Rayet stars in the galactic-centre field.
o	Table IV: <PN Al 2-A> (Nos 2-A to 2-S) N=19. Table V: <[A79] N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A80]
[A80]	(Arp, 1980)= (U)
Write:	<<[A80] NGC 2639 UNN>> <<[A80] NGC 2859 UN>>
N:	19+6
Object:	UV Obj. + QSO (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	1st ref.: N=19 Ultraviolet excess objects (Fig. 1), format 'NGC 2639 UNN' 10 are quasars (Nos U1-U5, U7, U8, U10, U14, U15). Identif. charts 2nd ref.: N=6 Ultraviolet excess objects, format 'NGC 2859 UN' 4 are quasars (Nos U1, U2, U3, U6)
Ref:	=1980ApJ...236...63A
by	ARP H.
	Astrophys. J., 236, 63-69 (1980)
	Ultraviolet excess objects in the region of a companion galaxy to NGC 2639.
o	<[A80] NGC 2639 UNN> (Nos 1-19)
Ref:	=1980ApJ...240..415A
by	ARP H.
	Astrophys. J., 240, 415-420 (1980)
	High-redshift objects near the companion galaxies to NGC 2859.
o	<[A80] NGC 2859 UN> (Nos U1-U6)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A81]
[A81]	(Arp, 1981)= ([A81a])
Write:	<<[A81] HHMMSS+DDMMAAA>>
N:	99
Object:	G + Part of G (SIMBAD class: Galaxy)
Note:	Table 1: N=72 galaxies, format 'HHMMSS+DDMM' and N=38 components of these galaxies, format 'HHMMSS+DDMMAAA' where the letters are often directions.
Ref:	=1981ApJS...46...75A
by	ARP H.
	Astrophys. J., Suppl. Ser., 46, 75-112 (1981)
	Spectroscopic measures of galaxies, their companions, and peculiar galaxies in the Southern Hemisphere.
o	In table 1, 1950 positions are measured positions, not those of the AM catalogue.
o	Table 1: <[A81] HHMMSS+DDMMAA> N=99
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A81a]
[A81a]	(Arp, 1981)
*****	Avoid the usage of [A81a], prefer [A81]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A81b]
[A81b]	(Arp, 1981)= ([A83]) = (B) = (BSO) = (RSO) = (U) = (UB)
Write:	<<[A81b] NGC NNNN UB NN>> <<[A81b] NGC NNNN BSO N>> <<[A81b] NGC NNNN RSO>> <<[A81b] NGC NNNN B N>> <<[A81b] NGC NNNN W1>>
N:	80
Object:	(Blue + UV) (SIMBAD class: blue = Blue Object)
Note:	N=62 (1st ref.) + 18 new (2nd ref.) Blue, UV, and UV-Blue objects, format NGC NNNN UB NN, or NGC NNNN BSO N, or NGC NNNN RSO, NGC NNNN W1 or NGC NNNN B N. Those among these objects who are QSO are in the tables
Ref:	=1981ApJ...250...31A
by	ARP H.
	Astrophys. J., 250, 31-42 (1981)
	Quasars near companion galaxies.
o	Companions galaxies are not in SIMBAD. 0846+51W1 = 6W 0846+51W1, 0959+68W1 = 6W 0959+68W1, Hoag 1 to 3 = [BJK80] 1 to 3
o	Table 1: <[A81b] NGC NNNN UB NN>, <[A81b] NGC NNNN BSO N>, <[A81b] NGC NNNN RSO>, <[A81b] NGC NNNN B N>, N=62.
Ref:	=1983ApJ...271..479A
by	ARP H.
	Astrophys. J., 271, 479-506 (1983)
	Further observations and analysis of quasars near companion galaxies.
o	Companions galaxies are not in SIMBAD.
o	Tables 5,6: [A83] use <[A81b] NGC NNNN UB NN> N=18 new. Table 5, Fig.7: <[BJK80] N> No. 4 is new
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A81c]
[A81c]	(Alcaino, 1981)
Write:	<<[A81c] A>>
N:	13
Object:	* (SIMBAD class: Star)
Note:	Photoelectric sequence of N=13 stars in the field of NGC 253.
in source:	NGC 253
Ref:	=1981A&A....97..201A
by	ALCAINO G.
	Astron. Astrophys., 97, 201-202 (1981)
	A photoelectric sequence in the region of the Sculptor Galaxy NGC 253.
o	Table 1: <[A81c] A> (Nos A-N).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A83]
[A83]	(Arp, 1983)
*****	Avoid the usage of [A83], prefer [A81b]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A84]
[A84]	(Arp, 1984)= (QSO)
Write:	<<[A84] QSO N>>
N:	2
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	Plate
in source:	NGC 3842
Ref:	=1984ApJ...283...59A
by	ARP H.
	Astrophys. J., 283, 59-63 (1984)
	Two newly discovered quasars closely spaced across a galaxy.
o	<[A84] QSO N> (Nos 1-2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A86]
[A86]	(Altschuler, 1986)
Write:	<<[A86] HHMM+DDdA>>
N:	882
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Ref:	=1986A&AS...65..267A
by	ALTSCHULER D.R.
	Astron. Astrophys., Suppl. Ser., 65, 267-283 (1986)
	A 5-GHz survey of radio sources.
o	<[A86] HHMM+DDdA> N=882
=E=	Catalogue in electronic form as J/A+AS/65/267
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A92]
[A92]	(Annis, 1992)
Write:	<<[A92] J1131+0456 A>> <<[A92] N>>
N:	4+8
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=4 (IR) components of MITG J1131+0456, (Nos A-D). Map in Fig.1. See also radio components [HTS88]. Table 2: N=8 faint objects around MITG. Map in Fig.3.
in source:	MITG J1131+0456
Ref:	=1992ApJ...391L..17A
by	ANNIS J.
	Astrophys. J., 391, 17-20 (1992)
	The unusual K-band characteristics of the gravitational lens system MG 1131+0456.
o	Fig.2: [HTS88] J1131+0456 A1 and A2.
o	Table 1: <[A92] J1131+0456 A> (Nos A-D). Table 2: <[A92] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A94]
[A94]	(Arp, 1994)= ([A94a])
Write:	<<[A94] NN>>
N:	56 among 66
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
in source:	Cen A = NGC 5128
Ref:	=1994A&A...288..738A
by	ARP H.
	Astron. Astrophys., 288, 738-745 (1994)
	ROSAT X-ray survey of an area 10 ° square around the active radio galaxy Centaurus A.
o	<[A94] NN> N=66
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A94a]
[A94a]	(Arp, 1994)
*****	Avoid the usage of [A94a], prefer [A94]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A95]
[A95]	(Arp, 1995)
Write:	<<[A95] a>>
N:	8
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Observed with ROSAT PSPC
Ref:	=1995A&A...296L...5A
by	ARP H.
	Astron. Astrophys., 296, 5-8 (1995)
	Alignment of radio and X-ray sources across PG 1211+143.
o	Table 1: <[A95] a> (Nos a-h) N=8
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A96]
[A96]	(Arp, 1996)
Write:	<<[A96] Mrk NNN NN>> <<[A96] Mrk NNN a>> <<[A96] NGC NNNN NN>> <<[A96] 3C 309.1 N>> <<[A96] 3C 309.1 a>> <<[A96] 3C 232 a>> <<[A96] 3C 232 a'>>
N:	129
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT PSPC, HRI observations. Table 2b: 'Mrk 474 NN' (Nos 1-25), (X) in the field of Mrk 474 (= [A96] Mrk 474 1). Table 3: 'Mrk 474 a' (Nos a-e), other (X) in the field of Mrk 474. Table 5: 'NGC 4651 NN' (Nos 1-24), (X) in the field of NGC 4651 (= [A96] NGC 4651 1). Table 6: 'NGC 3067 NN' (Nos 1-21), (X) in the field of NGC 3067. Table 8: 'Mrk 205 NN' (Nos 1-12, 18), (X) in the field of Mrk 205. Table 9: 'Mrk 205 a' (Nos a-c), poss. QSO. Table 10: '3C 309.1 N', (Nos 1-6), (X) in the field of 3C 309.1. Table 11: '3C 309.1 a' (Nos a-f), other (X) in the field of 3C 309.1. Table 12: '3C 232 a' and '3C 232 a'', (Nos a-f and a') (X) in the field of 3C 232
Ref:	=1996A&A...316...57A
by	ARP H.
	Astron. Astrophys., 316, 57-78 (1996)
	X-ray observations of five galaxy-quasar associations.
o	BSOI = QSO 1432+489
o	Tables 2b: <[A96] Mrk 474 NN> (Nos 1-25). Table 3: <[A96] Mrk 474 a>(Nos a-e). Table 5: <[A96] NGC 4651 NN> (Nos 1-24). Table 6: <[A96] NGC 3 067 NN > (Nos 1-21). Table 8: <[A96] Mrk 205 NN> (Nos 1-12, 18). Table 9: <[A96] Mrk 2 05 a> (Nos a-c). Table 10: <[A96] 3C 309.1 N> (Nos 1-6). Table 11: <[A96] 3C 30 9.1 a> (Nos a-f). Table 12: <[A96] 3C 232 a> (Nos a-f), <[A96] 3C 232 a'>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A97]
[A97]	(Arp, 1997)= ([A97a])
Write:	<<[A97] JHHMMSS.s+DDMMSS>>
N:	37
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	N=37 QSO around 3C 345
Ref:	=1997A&A...327..479A
by	ARP H.
	Astron. Astrophys., 327, 479-482 (1997)
	Concentration of quasars around the active extragalactic object 3C 345.
o	Table 1: <[A97] JHHMMSS.s+DDMMSS> N=37
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A97a]
[A97a]	(Arp, 1997)
*****	Avoid the usage of [A97a], prefer [A97]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A97b]
[A97b]	(Arp, 1997)
Write:	<<[A97b] 2-N>> <<[A97b] 3-N>> <<[A97b] JHHMMSS.s+DDMMSS>>
N:	3+4+8
Object:	* + (X) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 1, Fig.2: N=3 stars in the field of the BL Lac object '[A97b] 2-1', format '2-N'. Table 1, Fig.3: N=4 stars in the field of the QSO '[A97b] 3-1' = PG 1216+069, format '3-N'. Table 3: N=8 X-ray sources in the NE field of NGC 2639
Ref:	=1997A&A...328L..17A
by	ARP H.
	Astron. Astrophys., 328, 17-20 (1997)
	Pairs of X-ray sources across Seyferts: the NGC 4235 field.
o	Table 1, Fig.2: <[A97b] 2-N> (Nos 2-1 to 2-3), Table 1, Fig.3: <[A97b] 3-N> (Nos 3-1 to 3-4). Table 3: <[A97b] JHHMMSS.s+DDMMSS> N=8
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A97c]
[A97c]	(Arp, 1997)
Write:	<<[A97c] JHHMMSS.s+DDMMSS>>
N:	33
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Optical identification of ROSAT PSPC sources around 4 bright Seyfert galaxies. A few objects are also found in 1998ApJ.500.596C with the format [CWH98] JHHMM+DDMM See [CWH98]
in source:	NGC 4235
in source:	NGC 3516
in source:	NGC 5273
in source:	NGC 5548
Ref:	=1997A&A...319...33A
by	ARP H.
	Astron. Astrophys., 319, 33-44 (1997)
	Identification of X-ray sources <1° from Seyfert galaxies.
o	in table 1 NGC 1556 is a misprint for NGC 1566.
o	Table 3: <[A97c] JHHMMSS.s+DDMMSS> N=33.
=E=	Catalogue in electronic form as J/A+A/319/33
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A98]
[A98]	(Arp, 1998)= ([A98a])
Write:	<<[A98] NGC 2639 NE a>>
N:	7
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=7 X-ray sources NorthEast of NGC 2639
in source:	NGC 2639
Ref:	=1998ApJ...496..661A
by	ARP H.
	Astrophys. J., 496, 661-669 (1998)
	The origin of companion galaxies.
o	NGC 2639 U10 = [A80] NGC 2639 U10
o	Table 2: <[A98] NGC 2639 NE a> (Nos a-g).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A98a]
[A98a]	(Arp, 1998)
*****	Avoid the usage of [A98a], prefer [A98]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A98b]
[A98b]	(Aspin, 1998)= (AS) = (CA)
Write:	<<[A98b] N>>
N:	9
Object:	H2 Nebula (SIMBAD class: ISM = Interstellar Medium Object)
Stat:	is completely incorporated in Simbad
Note:	N=9 H2 nebulous objects in the field of AFGL 961 Map in Fig.1
Ref:	=1998A&A...335.1040A
by	ASPIN C.
	Astron. Astrophys., 335, 1040-1048 (1998)
	Discovery of multiple non-axially symmetric near-IR bow shocks around the pre-main sequence binary AFGL 961.
o	Table 1: <[A98b] N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [A99]
[A99]	(Arp, 1999)
Write:	<<[A99] PSPC NN>> <<[A99] HRI NN>> <<[A99] HRI a>> <<[A99] UV A>>
N:	49+12+1+6
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT PSPC and HRI observations of NGC 1097. Table I: PSPC objects in the field of NGC 1097, N=49. Table V: HRI objects in the field of NGC 1097, N=12 among (Nos 1-18). Fig.6: N=1 HRI source, No. 'a'. Fig.7: N=6 UV features in the HRI map.
in source:	NGC 1097
Ref:	=1999Ap&SS.262..337A
by	ARP H.
	Astrophys. Space Sci., 262, 337-361 (1999)
	X-ray observations of NGC 1097 and nearby quasars.
o	Table I: <[A99] PSPC NN> (Nos 1-49). Table V: <[A99] HRI NN> N=12 among (Nos 1-18). Fig.6: <[A99] HRI a> (No. a). Fig.7: <[A99] UV A> (Nos A-F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAA2003]
[AAA2003]	(Afonso+Albert+Alard+, 2003)
Write:	<<[AAA2003] NN>>
N:	16
Object:	Lensing Event (SIMBAD class: LensingEv = (Micro)Lensing Event)
Stat:	is completely incorporated in Simbad
Note:	EROS 2 observations of the Galactic Bulge searching for microlensing event candidates. See also EROS2-BLG.
Ref:	=2003A&A...404..145A
by	AFONSO C. , ALBERT J.N., ALARD C., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., BAUER F., BEAULIEU J.P., BLANC G., BOUQUET A., CHAR S., CHARLOT X., COUCHOT F., COUTURES C., DERUE F., FERLET R., FOUQUE P., GLICENSTEIN J.F., GOLDMAN B., GOULD A., GRAFF D., GROS M., HAISSINSKI J., HAMADACHE C., HAMILTON J.C., HARDIN D., DE KAT J., KIM A., LASSERRE T., LE GUILLOU L., LESQUOY E., LOUP C., MAGNEVILLE C., MANSOUX B., MARQUETTE J.B., MAURICE E., MAURY A., MILSZTAJN A., MONIEZ M., PALANQUE-DELABROUILLE N., PERDEREAU O., PREVOT L., REGNAULT N., RICH J., SPIRO M., TISSERAND P., VIDAL-MADJAR A., VIGROUX L., ZYLBERAJCH S.
	Astron. Astrophys., 404, 145-156 (2003)
	Bulge microlensing optical depth from EROS 2 observations.
o	These are EROS2 observations and thus they are called EROS2-BLG NN in Simbad and not EROS-BLG NN as proposed by the authors in the article. objects OGLE = EWS YYYY-AAA-NN, EROS YY-BLG NN = EROS BLG YYYY NN in Simbad.
o	Table 3: <[AAA2003] NN> (Nos 1-16) = <EROS2-BLG NN> N=16 among (Nos 2-35).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAA2010]
[AAA2010]	(Abdo+Ackermann+Ajello+, 2010) (Not yet in Simbad)
Write:	<<[AAA2010] SN>> <<[AAA2010] GN>>
N:	5+2
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	Fermi LAT observations of the LMC.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2010A&A...512A...7A
by	ABDO A.A. , ACKERMANN M., AJELLO M., ATWOOD W.B., BALDINI L., BALLET J., BARBIELLINI G., BASTIERI D., BAUGHMAN B.M., BECHTOL K., BELLAZZINI R., BERENJI B., BLANDFORD R.D., BLOOM E.D., BONAMENTE E., BORGLAND A.W., BREGEON J., BREZ A., BRIGIDA M., BRUEL P., BURNETT T.H., BUSON S., CALIANDRO G.A., CAMERON R.A., CARAVEO P.A., CASANDJIAN J.M., CECCHI C., CELIK O., CHEKHTMAN A., CHEUNG C.C., CHIANG J., CIPRINI S., CLAUS R., COHEN-TANUGI J., COMINSKY L.R., CONRAD J., CUTINI S., DERMER C.D., DE ANGELIS A., DE PALMA F., DIGEL S.W., DO COUTO E SILVA E., DRELL P.S., DUBOIS R., DUMORA D., FARNIER C., FAVUZZI C., FEGAN S.J., FOCKE W.B., FORTIN P., FRAILIS M., FUKAZAWA Y., FUSCO P., GARGANO F., GASPARRINI D., GEHRELS N., GERMANI S., GIAVITTO G., GIEBELS B., GIGLIETTO N., GIORDANO F., GLANZMAN T., GODFREY G., GOTTHELF E.V., GRENIER I.A., GRONDIN M.-H., GROVE J.E., GUILLEMOT L., GUIRIEC S., HANABATA Y., HARDING A.K., HAYASHIDA M., HAYS E., HORAN D., HUGHES R.E., JACKSON M.S., JEAN P., JOHANNESSON G., JOHNSON A.S., JOHNSON R.P., JOHNSON T.J., JOHNSON W.N., KAMAE T., KATAGIRI H., KATAOKA J., KAWAI N., KERR M., KNOEDLSEDER J., KOCIAN M.L., KUSS M., LANDE J., LATRONICO L., LEMOINE-GOUMARD M., LONGO F., LOPARCO F., LOTT B., LOVELLETTE M.N., LUBRANO P., MADEJSKI G.M., MAKEEV A., MARSHALL F., MARTIN P., MAZZIOTTA M.N., McCONVILLE W., McENERY J.E., MEURER C., MICHELSON P.F., MITTHUMSIRI W., MIZUNO T., MOISEEV A.A., MONTE C., MONZANI M.E., MORSELLI A., MOSKALENKO I.V., MURGIA S., NOLAN P.L., NORRIS J.P., NUSS E., OHSUGI T., OMODEI N., ORLANDO E., ORMES J.F., PANEQUE D., PARENT D., PELASSA V., PEPE M., PESCE-ROLLINS M., PIRON F., PORTER T.A., RAINO S., RANDO R., RAZZANO M., REIMER A., REIMER O., REPOSEUR T., RITZ S., RODRIGUEZ A.Y., ROMANI R.W., ROTH M., RYDE F., SADROZINSKI H.F.-W., SANCHEZ D., SANDER A., SAZ PARKINSON P.M., SCARGLE J.D., SELLERHOLM A., SGRO C., SISKIND E.J., SMITH D.A., SMITH P.D., SPANDRE G., SPINELLI P., STARCK J.-L., STRICKMAN M.S., STRONG A.W., SUSON D.J., TAJIMA H., TAKAHASHI H., TANAKA T., THAYER J.B., THAYER J.G., THOMPSON D.J., TIBALDO L., TORRES D.F., TOSTI G., TRAMACERE A., UCHIYAMA Y., USHER T.L., VASILEIOU V., VENTER C., VILCHEZ N., VITALE V., WAITE A.P., WANG P., WELTEVREDE P., WINER B.L., WOOD K.S., YLINEN T., ZIEGLER M.
	Astron. Astrophys., 512A, 7-7 (2010)
	Observations of the Large Magellanic Cloud with Fermi.
o	Table 2: <[AAA2010] SN> (Nos S1-S5). Table 3: <[AAA2010] GN> (Nos G1-G2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAA2011]
[AAA2011]	(Abdo+Ackermann+Ajello+, 2011)
Write:	<<[AAA2011] A>>
N:	3
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Fermi LAT observations of the field of RX J1713.7-3946.
in source:	RX J1713.0-3946
Ref:	=2011ApJ...734...28A
by	ABDO A.A. , ACKERMANN M., AJELLO M., ALLAFORT A., BALDINI L., BALLET J., BARBIELLINI G., BARING M.G., BASTIERI D., BELLAZZINI R., BERENJI B., BLANDFORD R.D., BLOOM E.D., BONAMENTE E., BORGLAND A.W., BOUVIER A., BRANDT T.J., BREGEON J., BRIGIDA M., BRUEL P., BUEHLER R., BUSON S., CALIANDRO G.A., CAMERON R.A., CARAVEO P.A., CASANDJIAN J.M., CECCHI C., CHATY S., CHEKHTMAN A., CHEUNG C.C., CHIANG J., CILLIS A.N., CIPRINI S., CLAUS R., COHEN-TANUGI J., CONRAD J., CORBEL S., CUTINI S., DE ANGELIS A., DE PALMA F., DERMER C.D., DIGEL S.W., DO COUTO E SILVA E., DRELL P.S., DRLICA-WAGNER A., DUBOIS R., DUMORA D., FAVUZZI C., FERRARA E.C., FORTIN P., FRAILIS M., FUKAZAWA Y., FUKUI Y., FUNK S., FUSCO P., GARGANO F., GASPARRINI D., GEHRELS N., GERMANI S., GIGLIETTO N., GIORDANO F., GIROLETTI M., GLANZMAN T., GODFREY G., GRENIER I.A., GRONDIN M.-H., GUIRIEC S., HADASCH D., HANABATA Y., HARDING A.K., HAYASHIDA M., HAYASHI K., HAYS E., HORAN D., JACKSON M.S., JOHANNESSON G., JOHNSON A.S., KAMAE T., KATAGIRI H., KATAOKA J., KERR M., KNODLSEDER J., KUSS M., LANDE J., LATRONICO L., LEE S.-H., LEMOINE-GOUMARD M., LONGO F., LOPARCO F., LOVELLETTE M.N., LUBRANO P., MADEJSKI G.M., MAKEEV A., MAZZIOTTA M.N., McENERY J.E., MICHELSON P.F., MIGNANI R.P., MITTHUMSIRI W., MIZUNO T., MOISEEV A.A., MONTE C., MONZANI M.E., MORSELLI A., MOSKALENKO I.V., MURGIA S., NAUMANN-GODO M., NOLAN P.L., NORRIS J.P., NUSS E., OHSUGI T., OKUMURA A., ORLANDO E., ORMES J.F., PANEQUE D., PARENT D., PELASSA V., PESCE-ROLLINS M., PIERBATTISTA M., PIRON F., POHL M., PORTER T.A., RAINO S., RANDO R., RAZZANO M., REIMER O., REPOSEUR T., RITZ S., ROMANI R.W., ROTH M., SADROZINSKI H.F.-W., SAZ PARKINSON P.M., SGRO C., SMITH D.A., SMITH P.D., SPANDRE G., SPINELLI P., STRICKMAN M.S., TAJIMA H., TAKAHASHI H., TAKAHASHI T., TANAKA T., THAYER J.G., THAYER J.B., THOMPSON D.J., TIBALDO L., TIBOLLA O., TORRES D.F., TOSTI G., TRAMACERE A., TROJA E., UCHIYAMA Y., VANDENBROUCKE J., VASILEIOU V., VIANELLO G., VILCHEZ N., VITALE V., WAITE A.P., WANG P., WINER B.L., WOOD K.S., YAMAMOTO H., YAMAZAKI R., YANG Z., ZIEGLER M.
	Astrophys. J., 734, 28 (2011)
	Observations of the young supernova remnant RX J1713.7-3946 with the Fermi large area telescope.
o	Figs 1-2, Table 2: <[AAA2011] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAA2018]
[AAA2018]	(Abeysekara+Archer+Aune+, 2018)
Write:	<<[AAA2018] FGL JHHMM.m+DDMM>> <<[AAA2018] FGL J2032.2+4128e>>
N:	24+1
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	N=25 gamma-ray point sources identified in Fermi LAT count maps of the Cygnus region.
in source:	NAME Cyg Region
Ref:	=2018ApJ...861..134A
by	ABEYSEKARA A.U. , ARCHER A., AUNE T., BENBOW W., BIRD R., BROSE R., BUCHOVECKY M., BUGAEV V., CUI W., DANIEL M.K., FALCONE A., FENG Q., FINLEY J.P., FLEISCHHACK H., FLINDERS A., FORTSON L., FURNISS A., GOTTHELF E.V., GRUBE J., HANNA D., HERVET O., HOLDER J., HUANG K., HUGHES G., HUMENSKY T.B., HUTTEN M., JOHNSON C.A., KAARET P., KAR P., KELLEY-HOSKINS N., KERTZMAN M., KIEDA D., KRAUSE M., KUMAR S., LANG M.J., LIN T.T.Y., MAIER G., McARTHUR S., MORIARTY P., MUKHERJEE R., O'BRIEN S., ONG R.A., OTTE A.N., PANDEL D., PARK N., PETRASHYK A., POHL M., POPKOW A., PUESCHEL E., QUINN J., RAGAN K., REYNOLDS P.T., RICHARDS G.T., ROACHE E., ROUSSELLE J., RULTEN C., SADEH I., SANTANDER M., SEMBROSKI G.H., SHAHINYAN K., TYLER J., VASSILIEV V.V., WAKELY S.P., WARD J.E., WEINSTEIN A., WELLS R.M., WILCOX P., WILHELM A., WILLIAMS D.A., ZITZER B.
	Astrophys. J., 861, 134-134 (2018)
	A very high energy γ-ray survey toward the Cygnus region of the Galaxy.
o	Tables 1+3: <[AAA2018] FGL JHHMM.m+DDMM> N=24, <[AAA2018] FGL J2032.2+4128e> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAA2019]
[AAA2019]	(Aksaker+Akyuz+Avdan+, 2019)
Write:	<<[AAA2019] A>>
N:	4
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=4 optical sources as possible counterparts of the ultraluminous X-ray source (ULX) X-1 in NGC 2500, using HST WFC3/UVIS archival images.
in source:	NGC 2500
Ref:	=2019MNRAS.488.5935A
by	AKSAKER N. , AKYUZ A., AVDAN S., AVDAN H.
	Mon. Not. R. Astron. Soc., 488, 5935-5940 (2019)
	Optical counterparts of an ultraluminous X-Ray Source X-1 in NGC 2500.
o	Fig. 2, Table 2: <[AAA2019] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAA2020]
[AAA2020]	(Albert+Alfaro+Alvarez+, 2020)
Write:	<<[AAA2020] PS J2005.0+3419>>
N:	1
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	HAWC and Fermi LAT observations of N=1 point source in the field 2HWC J2006+341.
Ref:	=2020ApJ...903L..14A
by	ALBERT A. , ALFARO R., ALVAREZ C., ANGELES CAMACHO J.R., ARAYA M., ARTEAGA-VELAZQUEZ J.C., ARUNBABU K.P., AVILA ROJAS D., AYALA SOLARES H.A., BAGHMANYAN V., BELMONT-MORENO E., BRISBOIS C., CABALLERO-MORA K.S., CARRAMINANA A., CASANOVA S., COTTI U., DE LA FUENTE E., DE LEON C., DIAZ HERNANDEZ R., DINGUS B.L., DUVERNOIS M.A., DUROCHER M., DIAZ-VELEZ J.C., ESPINOZA C., FLEISCHHACK H., FRAIJA N., GALVAN-GAMEZ A., GARCIA D., GARCIA-GONZALEZ J.A., GARFIAS F., GONZALEZ M.M., GOODMAN J.A., HARDING J.P., HONA B., HUANG D., HUEYOTL-ZAHUANTITLA F., HUNTEMEYER P., IRIARTE A., JARDIN-BLICQ A., JOSHI V., LEON VARGAS H., LINNEMANN J.T., LONGINOTTI A.L., LOPEZ-COTO R., LUIS-RAYA G., LUNDEEN J., MALONE K., MARTINEZ O., MARTINEZ-CASTRO J., MATTHEWS J.A., MIRANDA-ROMAGNOLI P., MORENO E., MOSTAFA M., NELLEN L., NISA M.U., NORIEGA-PAPAQUI R., OMODEI N., PEISKER A., PEREZ-PEREZ E.G., RHO C.D., ROSA-GONZALEZ D., SALESA GREUS F., SANDOVAL A., SCHNEIDER M., SPRINGER R.W., TOLLEFSON K., TORRES I., TORRES-ESCOBEDO R., URENA-MENA F., VILLASENOR L., WEISGARBER T., WILLOX E., ZEPEDA A., ZHOU H., (The HAWC Collaboration)
	Astrophys. J., 903L, 14-14 (2020)
	HAWC and Fermi-LAT detection of extended emission from the unidentified source 2HWC J2006+341.
o	Fig. 1: <[AAA2020] PS J2005.0+3419> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAA95]
[AAA95]	(Alcock+Allsman+Axelrod+, 1995)
Write:	<<[AAA95] JHHMMSS.s+DDMMSS>>
N:	48
Object:	* (SIMBAD class: Cepheid = Cepheid Variable)
Stat:	is completely incorporated in Simbad
Note:	MACHO project. Finding Charts in Plates 60-63 See also MACHO*
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1995AJ....109.1653A
by	ALCOCK C. , ALLSMAN R.A., AXELROD T.S., BENNETT D.P., COOK K.H., FREEMAN K.C., GRIEST K., MARSHALL S.L., PETERSON B.A., PRATT M.R., QUINN P.J., REIMANN J., RODGERS A.W., STUBBS C.W., SUTHERLAND W., WELCH D.L.
	Astron. J., 109, 1653-1662 (1995)
	The MACHO project LMC variable star inventory. I. Beat Cepheids-conclusive evidence for the excitation of the second overtone in classical Cepheids.
o	Table 1 : * HS 353 not identified
o	Table 1: <MACHO* JHHMMSS.s-DDMMSS> = <[AAA95] JHHMMSS.s-DDMMSS> N=48
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAA97a]
[AAA97a]	(Alcock+Allsman+Alves+, 1997)
Write:	<<[AAA97a] JHHMMSS.ss+DDMMSS.s>>
N:	30
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Stat:	is completely incorporated in Simbad
Note:	MACHO project. See also MACHO*
in source:	NAME SDG = NAME Sgr Dwarf Galaxy
Ref:	=1997ApJ...474..217A
by	ALCOCK C. , ALLSMAN R.A., ALVES D.R., AXELROD T.S., BECKER A.C., BENNETT D.P., COOK K.H., FREEMAN K.C., GRIEST K., GUERN J.A., LEHNER M.J., MARSHALL S.L., MINNITI D., PETERSON B.A., PRATT M.R., QUINN P.J., RODGERS A.W., STUBBS C.W., SUTHERLAND W., WELCH D.L., (The MACHO Collaboration)
	Astrophys. J., 474, 217-None (1997)
	MACHO project photometry of RR Lyrae stars in the Sagittarius dwarf galaxy.
o	Table 1: <[AAA97a] JHHMMSS.ss+DDMMSS.s> = <MACHO* JHHMMSS.ss+DDMMSS.s> = <MACHO* FFFNNNN> N=30
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAA97b]
[AAA97b]	(Alcock+Allsman+Alves+, 1997)
Write:	<<[AAA97b] JHHMMSS.s+DDMMSS>>
N:	611
Object:	Binary * (SIMBAD class: EclBin = Eclipsing Binary)
Stat:	is completely incorporated in Simbad
Note:	MACHO project. See also MACHO*
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1997AJ....114..326A
by	ALCOCK C. , ALLSMAN R.A., ALVES D., AXELROD T.S., BECKER A.C., BENNETT D.P., COOK K.H., FREEMAN K.C., GRIEST K., LACY C.H.S., LEHNER M.J., MARSHALL S.L., MINITI D., PETERSON B.A., PRATT M.R., QUINN P.J., RODGERS A.W., STUBBS C.W., SUTHERLAND W., WELCH D.L.
	Astron. J., 114, 326-None (1997)
	The MACHO project LMC variable star inventory. V. Classification and orbits of 611 eclipsing binary stars.
o	Table 1: cross-id. with 'MACHO* JHHMMSS.ss+DDMMSS.s'
o	Table 1: <[AAA97b] JHHMMSS.s-DDMMSS> N=611
=E=	Catalogue in electronic form as J/AJ/114/326
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAA97c]
[AAA97c]	(Alcock+Allsman+Alves+, 1997)
Write:	<<[AAA97c] JHHMMSS.s+DDMMSS>>
N:	73
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Stat:	is completely incorporated in Simbad
Note:	MACHO project. Table 1: N=75 entries but two pairs represent the same stars found twice in overlapping regions of different MACHO fields. See also MACHO*
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1997ApJ...482...89A
by	ALCOCK C. , ALLSMAN R.A., ALVES D., AXELROD T.S., BECKER A.C., BENNETT D.P., COOK K.H., FREEMAN K.C., GRIEST K., GUERN J., LEHNER M.J., MARSHALL S.L., MINNITI D., PETERSON B.A., PRATT M.R., QUINN P.J., RODGERS A.W., SUTHERLAND W., WELCH D.L., (The MACHO Collaboration)
	Astrophys. J., 482, 89-97 (1997)
	The MACHO project Large Magellanic Cloud variable star inventory. III. Multimode RR Lyrae stars, distance to the large Magellanic Cloud, and age of the oldest stars.
o	Table 1: N=75 entries, but N=73 RRLyr, two pairs represent the same stars found twice.
o	Table 1: <[AAA97c] JHHMMSS.s-DDMMSS> = <MACHO* JHHMMSS.s-DDMMSS> = <MACHO FFF.NNNNN.NNNN> N=75
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAA97d]
[AAA97d]	(Alcock+Allsman+Alves+, 1997)
Write:	<<[AAA97d] JHHMMSS.sss+DDMMSS.ss>>
N:	20
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Stat:	is completely incorporated in Simbad
Note:	MACHO project. See also MACHO*
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1997ApJ...490L..59A
by	ALCOCK C. , ALLSMAN R.A., ALVES D.R., AXELROD T.S., BECKER A.C., BENNETT D.P., COOK K.H., FREEMAN K.C., GRIEST K., LEHNER M.J., MARSHALL S.L., MINNITI D., PETERSON B.A., PRATT M.R., QUINN P.J., RODGERS A.W., RORABECK A., STUBBS C.W., SUTHERLAND W., TOMANEY A.B., VANDEHEI T., WELCH D.L.
	Astrophys. J., 490, 59-64 (1997)
	Is the Large Magellanic Cloud microlensing due to an intervening dwarf galaxy?
o	Table 1: <[AAA97d] JHHMMSS.sss+DDMMSS.ss> = <MACHO* JHHMMSS.sss+DDMMSS.ss> N=20
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAA98a]
[AAA98a]	(Alcock+Allsman+Alves+, 1998)
Write:	<<[AAA98a] JHHMMSS.ssss+DDMMSS.sss>>
N:	20
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Stat:	is completely incorporated in Simbad
Note:	MACHO project. See also MACHO*
Ref:	=1998ApJ...494..396A
by	ALCOCK C. , ALLSMAN R.A., ALVES D.R., AXELROD T.S., BECKER A.C., BENNETT D.P., COOK K.H., FREEMAN K.C., GRIEST K., GOULD A., GUERN J.A., LEHNER M.J., MARSHALL S.L., MINNITI D., PETERSON B.A., POPOWSKI P., PRATT M.R., QUINN P.J., RODGERS A.W., STUBBS C.W., SUTHERLAND W., VANDEHEI T., WELCH D.L., (The MACHO Collaboration)
	Astrophys. J., 494, 396-399 (1998)
	The zero point of extinction toward Baade's Window from RR Lyrae stars.
o	Table 1: <[AAA98a] JHHMMSS.ssss+DDMMSS.sss> = <MACHO* JHHMMSS.ssss+DDMMSS.sss>, N=20
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAA98b]
[AAA98b]	(Alcock+Allsman+Alves+, 1998)
Write:	<<[AAA98b] JHHMMSS.s+DDMMSS>>
N:	33
Object:	Pulsating V* (SIMBAD class: PulsV* = Pulsating Variable)
Stat:	is completely incorporated in Simbad
Note:	MACHO project. See also MACHO*
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1998AJ....115.1921A
by	ALCOCK C. , ALLSMAN R.A., ALVES D.R., AXELROD T.S., BECKER A., BENNETT D.P., COOK K.H., FREEMAN K.C., GRIEST K., LAWSON W.A., LEHNER M.J., MARSHALL S.L., MINNITI D., PETERSON B.A., POLLARD K.R., PRATT M.R., QUINN P.J., RODGERS A.W., SUTHERLAND W., TOMANEY A., WELCH D.L.
	Astron. J., 115, 1921-1933 (1998)
	The MACHO project LMC variable star inventory. VII. The discovery of RV Tauri stars and new type II cepheids in the Large Magellanic Cloud.
o	Table 1: The format 'FFF.NNNNN.NNNN' stands for 'MACHO FFF.NNNNN.NNNN' in SIMBAD.
o	Table 1: <MACHO* JHHMMSS.s+DDMMSS> = <[AAA98b] JHHMMSS.s+DDMMSS>, N=33.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAB2004]
[AAB2004]	(Arbour+Armstrong+Boles+, 2004)
Write:	<<[AAB2004] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of SN 2004EN.
Ref:	=2004IAUC.8406....1A
by	ARBOUR R. , ARMSTRONG M., BOLES T., ITAGAKI K., NAKANO S., MOORE M., LI W., BRIGGS D.
	IAU Circ., 8406, 1-None (2004)
	Supernovae 2004el, 2004em, 2004en, 2004eo, 2004ep.
o	<[AAB2004] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAB2005]
[AAB2005]	(Aharonian+Akhperjanian+Beilicke+, 2005) (Not yet in Simbad)
Write:	<<[AAB2005] SS 433 knot N>>
N:	2
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	TeV gamma-ray observations of SS 433: Knots 2 and 3 are in western lobe. See also [SO97], PVF99].
in source:	SS 433
Ref:	=2005A&A...439..635A
by	AHARONIAN F. , AKHPERJANIAN A., BEILICKE M., BERNLOEHR K., BOERST H.-G., BOJAHR H., BOLZ O., COARASA T., CONTRERAS J., CORTINA J., DENNINGHOFF S., FONSECA V., GIRMA M., GOETTING N., HEINZELMANN G., HERMANN G., HEUSLER A., HOFMANN W., HORNS D., JUNG I., KANKANYAN R., KESTEL M., KOHNLE A., KONOPELKO A., KRANICH D., LAMPEITL H., LOPEZ M., LORENZ E., LUCARELLI F., MANG O., MAZIN D., MEYER H., MIRZOYAN R., MORALEJO A., ONA-WILHELMI E., PANTER M., PLYASHESHNIKOV A., PUEHLHOFER G., DE LOS REYES R., RHODE W., RIPKEN J., ROWELL G.P., SAHAKIAN V., SAMORSKI M., SCHILLING M., SIEMS M., SOBZYNSKA D., STAMM W., TLUCZYKONT M., VITALE V., VOELK H.J., WIEDNER C.A., WITTEK W.
	Astron. Astrophys., 439, 635-643 (2005)
	TeV γ-ray observations of SS-433 and a survey of the surrounding field with the HEGRA IACT-System.
o	In Abstract GEV J1907+0537 is a probable misprint for GEV J1907+0557.
o	Table 3, Fig.3: <[AAB2005] SS 433 Knot N> (Nod 2, 3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAB2007]
[AAB2007]	(Abdo+Allen+Berley+, 2007)
Write:	<<[AAB2007] CN>>
N:	4
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Milagro Gamma-Ray Observatory TeV observations of the Galactic Plane: N=4 source candidates. See also MGRO.
Ref:	=2007ApJ...664L..91A
by	ABDO A.A. , ALLEN B., BERLEY D., CASANOVA S., CHEN C., COYNE D.G., DINGUS B.L., ELLSWORTH R.W., FLEYSHER L., FLEYSHER R., GONZALEZ M.M., GOODMAN J.A., HAYS E., HOFFMAN C.M., HOPPER B., HUNTEMEYER P.H., KOLTERMAN B.E., LANSDELL C.P., LINNEMANN J.T., McENERY J.E., MINCER A.I., NEMETHY P., NOYES D., RYAN J.M., SAZ PARKINSON P.M., SHOUP A., SINNIS G., SMITH A.J., SULLIVAN G.W., VASILEIOU V., WALKER G.P., WILLIAMS D.A., XU X.W., YODH G.B.
	Astrophys. J., 664L, 91-94 (2007)
	TeV γ-ray sources from a survey of the galactic plane with Milagro.
o	Table 2: <[AAB2007] CN> (Nos C1-C4). Table 2: <MGRO JHHMM+DD> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAB2008]
[AAB2008]	(Ahironian+Akhperjian+Barres de Almeida+, 2008)= ([AAB2008a])
Write:	<<[AAB2008] NN>>
N:	18
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS observations of the region of CTB 37b.
Ref:	=2008A&A...486..829A
by	AHARONIAN F. , AKHPERJANIAN A.G., BARRES DE ALMEIDA U., BAZER-BACHI A.R., BEHERA B., BEILICKE M., BENBOW W., BERNLOEHR K., BOISSON C., BORREL V., BRAUN I., BRION E., BRUCKER J., BUEHLER R., BULIK T., BUESCHING I., BOUTELIER T., CARRIGAN S., CHADWICK P.M., CHAVES R.C.G., CHOUNET L.-M., CLAPSON A.C., COIGNET G., CORNILS R., COSTAMANTE L., DALTON M., DEGRANGE B., DICKINSON H.J., DJANNATI-ATAIE A., DOMAINKO W., DRURY L.O'C., DUBOIS F., DUBUS G., DYKS J., EGBERTS K., EMMANOULOPOULOS D., ESPIGAT P., FARNIER C., FEINSTEIN F., FIASSON A., FOERSTER A., FONTAINE G., FUNK S., FUESSLING M., GABICI S., GALLANT Y.A., GIEBELS B., GLICENSTEIN J.F., GLUECK B., GORET P., HADJICHRISTIDIS C., HAUSER D., HAUSER M., HEINZELMANN G., HENRI G., HERMANN G., HINTON J.A., HOFFMANN A., HOFMANN W., HOLLERAN M., HOPPE S., HORNS D., JACHOLKOWSKA A., DE JAGER O.C., JUNG I., KATARZYNSKI K., KAUFMANN S., KENDZIORRA E., KERSCHHAGGL M., KHANGULYAN D., KHELIFI B., KEOGH D., KOMIN N., KOSACK K., LAMANNA G., LATHAM I.J., LEMOINE-GOUMARD M., LENAIN J.-P., LOHSE T., MARTIN J.M., MARTINEAU-HUYNH O., MARCOWITH A., MASTERSON C., MAURIN D., McCOMB T.J.L., MODERSKI R., MOULIN E., NAUMANN-GODO M., DE NAUROIS M., NEDBAL D., NEKRASSOV D., NOLAN S.J., OHM S., OLIVE J.-P., DE ONA WILHELMI E., ORFORD K.J., OSBORNE J.L., OSTROWSKI M., PANTER M., PEDALETTI G., PELLETIER G., PETRUCCI P.-O., PITA S., PUEHLHOFER G., PUNCH M., QUIRRENBACH A., RAUBENHEIMER B.C., RAUE M., RAYNER S.M., RENAUD M., RIEGER F., REIMER O., RIPKEN J., ROB L., ROSIER-LEES S., ROWELL G., RUDAK B., RUPPEL J., SAHAKIAN V., SANTANGELO A., SCHLICKEISER R., SCHOECK F.M., SCHROEDER R., SCHWANKE U., SCHWARZBURG S., SCHWEMMER S., SHALCHI A., SKILTON J.L., SOL H., SPANGLER D., STAWARZ L., STEENKAMP R., STEGMANN C., SUPERINA G., TAM P.H., TAVERNET J.-P., TERRIER R., VAN ELDIK C., VASILEIADIS G., VENTER C., VIALLE J.P., VINCENT P., VIVIER M., VOELK H.J., VOLPE F., WAGNER S.J., WARD M., ZDZIARSKI A.A., ZECH A.
	Astron. Astrophys., 486, 829-836 (2008)
	Chandra and HESS observations of the supernova remnant CTB37B.
o	Table 1: <[AAB2008] NN> (Nos 1-18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAB2008a]
[AAB2008a]	(Ahironian+Akhperjian+Barres de Almeida+, 2008)
*****	Avoid the usage of [AAB2008a], prefer [AAB2008]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAB2008b]
[AAB2008b]	(Aharonian+Akhperjanian+Bazer-Bachi+, 2008)
Write:	<<[AAB2008b] northeastern cloud>> <<[AAB2008b] southern cloud>>
N:	2
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	NANTEN 12CO(J=1-0) observations of N=2 molecular clouds in the W28 field. Use of the NANTEN Galactic Plane Survey data.
in source:	W 28
Ref:	=2008A&A...481..401A
by	AHARONIAN F. , AKHPERJANIAN A.G., BAZER-BACHI A.R., BEHERA B., BEILICKE M., BENBOW W., BERGE D., BERNLOEHR K., BOISSON C., BOLZ O., BORREL V., BRAUN I., BRION E., BROWN A.M., BUEHLER R., BULIK T., BUESCHING I., BOUTELIER T., CARRIGAN S., CHADWICK P.M., CHOUNET L.-M., CLAPSON A.C., COIGNET G., CORNILS R., COSTAMANTE L., DEGRANGE B., DICKINSON H.J., DJANNATI-ATAIE A., DOMAINKO W., DRURY L.O'C., DUBUS G., DYKS J., EGBERTS K., EMMANOULOPOULOS D., ESPIGAT P., FARNIER C., FEINSTEIN F., FIASSON A., FOERSTER A., FONTAINE G., FUKUI Y., FUNK SEB., FUNK S., FUESSLING M., GALLANT Y.A., GIEBELS B., GLICENSTEIN J.F., GLUECK B., GORET P., HADJICHRISTIDIS C., HAUSER D., HAUSER M., HEINZELMANN G., HENRI G., HERMANN G., HINTON J.A., HOFFMANN A., HOFMANN W., HOLLERAN M., HOPPE S., HORNS D., JACHOLKOWSKA A., DE JAGER O.C., KENDZIORRA E., KERSCHHAGGL M., KHELIFI B., KOMIN N., KOSACK K., LAMANNA G., LATHAM I.J., LE GALLOU R., LEMIERE A., LEMOINE-GOUMARD M., LENAIN J.-P., LOHSE T., MARTIN J.M., MARTINEAU-HUYNH O., MARCOWITH A., MASTERSON C., MAURIN G., McCOMB T.J.L., MODERSKI R., MORIGUCHI Y., MOULIN E., DE NAUROIS M., NEDBAL D., NOLAN S.J., OLIVE J.-P., ORFORD K.J., OSBORNE J.L., OSTROWSKI M., PANTER M., PEDALETTI G., PELLETIER G., PETRUCCI P.-O., PITA S., PUEHLHOFER G., PUNCH M., RANCHON S., RAUBENHEIMER B.C., RAUE M., RAYNER S.M., REIMER O., RENAUD M., RIPKEN J., ROB L., ROLLAND L., ROSIER-LEES S., ROWELL G., RUDAK B., RUPPEL J., SAHAKIAN V., SANTANGELO A., SAUGE L., SCHLENKER S., SCHLICKEISER R., SCHROEDER R., SCHWANKE U., SCHWARZBURG S., SCHWEMMER S., SHALCHI A., SOL H., SPANGLER D., STAWARZ L., STEENKAMP R., STEGMANN C., SUPERINA G., TAKEUCHI T., TAM P.H., TAVERNET J.-P., TERRIER R., VAN ELDIK C., VASILEIADIS G., VENTER C., VIALLE J.P., VINCENT P., VIVIER M., VOELK H.J., VOLPE F., WAGNER S.J., WARD M.
	Astron. Astrophys., 481, 401-410 (2008)
	Discovery of very high energy γ-ray emission coincident with molecular clouds in the W 28 (G6.4-0.1) field.
o	Figs, Table 1: <HESS JHHMM+DDdA> (Nos J1800-240A to C). Paragr. 3.: <[AAB2008b] northeastern cloud>, <[AAB2008b] southern cloud>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAF2013]
[AAF2013]	(Atkinson+Abraham+Ferguson, 2013) (Not yet in Simbad)
Write:	<<[AAF2013] WN-NNNN>>
N:	1780
Object:	G (SIMBAD class: Galaxy)
Note:	N=1780 galaxies from the wide-field component of the Canada-France-Hawaii Telescope Legacy Survey (CFHTLS).
Ref:	=2013ApJ...765...28A
by	ATKINSON A.M. , ABRAHAM R.G., FERGUSON A.M.N.
	Astrophys. J., 765, 28 (2013)
	Faint tidal features in galaxies within the Canada-France-Hawaii Telescope Legacy Survey wide fields.
o	Table 4: <[AAF2013] WN-NNNN> N=1780 among (Nos W1-2 to W1-806, W2-1 to W2-400, W3-2 to W3-934, W4-1 to W4-458).
=E=	Catalogue in electronic form as <J/ApJ/765/28/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAG2011]
[AAG2011]	(Alves+Acosta-Pulido+Girart+, 2011)
Write:	<<[AAG2011] NN>>
N:	34
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	WHT LIRIS 4.2-m telescope (NIR) and Pico dos Dias Observatory 1.6-m telescope (optical) linear polarimetry of N=34 stars in the star-forming region [JCC87] IRAS 4A.
in source:	NGC 1333:[JCC87] IRAS 4A = [JCC87] IRAS 4
Ref:	=2011AJ....142...33A
by	ALVES F.O. , ACOSTA-PULIDO J.A., GIRART J.M., FRANCO G.A.P., LOPEZ R.
	Astron. J., 142, 33 (2011)
	Infrared and optical polarimetry around the low-mass star-forming region NGC 1333 IRAS 4A.
o	Table 5: <[AAG2011] NN> (Nos 1-34).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAH2014]
[AAH2014]	(Abrahamyan+Andreasyan+Hovhannisyan+, 2014)
Write:	<<[AAH2014] NN>>
N:	25
Object:	Radio G (SIMBAD class: RadioG = Radio Galaxy)
Note:	N=26 scintillating radio galaxies detected at 102 MHz in field II of the Cambridge 7C list. Use of VLA FIRST data.
Ref:	=2014Ap.....57..359A
by	ABRAHAMYAN H.V. , ANDREASYAN R.R., HOVHANNISYAN M.A., PARONYAN G.M.
	Ap, 57, 359-369 (2014)
	Study of compact radio galaxies in the 7C II field.
o	A translation of Astrofizika Vol. 57, No 3, pp. 389-399, 2014
o	Table 2: <[AAH2014] NN> N=25.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAH75]
[AAH75]	(Ambartsumyan+Arp+Hoag+, 1975) (Not yet in Simbad)
Write:	<<[AAH75] Anon NN>>
N:	13
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	N=13 galaxies in the group designated as 'Anon', but found as being 'ZwCl 1449+6809' later.
in source:	ZwCl 1449+6809
Ref:	=1975Afz....11..193A
by	AMBARTSUMYAN V.A. , ARP H.C., HOAG A.A., MIRZOYAN L.V.
	Astrofizika, 11, 193-206 (1975)
	Some remarks on compact groups of compact galaxies.
o	Anon = ZwCl 1449+6809
o	Fig.1: <[AAH75] Anon NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAJ2015]
[AAJ2015]	(Anderson+Armentrout+Johnstone+, 2015)
Write:	<<[AAJ2015] GLLL.lll+BB.bbb>>
N:	264
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	GBT X-band hydrogen recombination line and continuum detections of N=264 WISE HII region candidates in the zone 225°≥l≥-20°, \|b\|≤6°. See also HRDS.
Ref:	=2015ApJS..221...26A
by	ANDERSON L.D. , ARMENTROUT W.P., JOHNSTONE B.M., BANIA T.M., BALSER D.S., WENGER T.V., CUNNINGHAM V.
	Astrophys. J., Suppl. Ser., 221, 26 (2015)
	Finding distant galactic HII regions.
o	Table 2: <[AAJ2015] GLLL.lll+BB.bbb> N=264.
=E=	Catalogue in electronic form as J/ApJS/221/26
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAK2003]
[AAK2003]	(Alcaino+Alvarado+Kurtev, 2003) (Not yet in Simbad)
Write:	<<[AAK2003] xxxx.xx-yyyy.yy>>
N:	1687
Object:	* in Cl* (SIMBAD class: Star)
Note:	New CCD photometry of the SMC star cluster 'Cl Lindsay 1'.
in source:	Magellanic Clouds:SMC:Cl Lindsay 1 = Cl Lindsay 1
Ref:	=2003A&A...407..919A
by	ALCAINO G. , ALVARADO F., KURTEV R.
	Astron. Astrophys., 407, 919-924 (2003)
	The SMC star cluster Lindsay 1. First UI photometric study.
o	Table 1: <[AAK2003] xxxx.xx-yyyy.yy> N=1637.
=E=	Catalogue in electronic form as J/A+A/407/919
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAL2018]
[AAL2018]	(Anderson+Armentrout+Luisi+, 2018)
Write:	<<[AAL2018] GLLL.lll+BB.bbb>>
N:	148
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	GBT observations of N=148 HII angularly large Galactic HII regions in radio recombination line (RRL) emission. See also HRDS, [ABB2014].
Ref:	=2018ApJS..234...33A
by	ANDERSON L.D. , ARMENTROUT W.P., LUISI M., BANIA T.M., BALSER D.S., WENGER T.V.
	Astrophys. J., Suppl. Ser., 234, 33-33 (2018)
	A Green Bank Telescope Survey of large Galactic H II regions.
o	Table 1: <[AAL2018] GLLL.lll+BB.bbb> N=148.
=E=	Catalogue in electronic form as <J/ApJS/234/33/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AAO
AAO	(Abatsumani Astrophys. Obs.)
Write:	<<AAO +DD NNN>>
N:	6037
Object:	* (SIMBAD class: Star)
Note:	Catalog: format +DD NNN. zone Dec +23deg to +35deg Identif. charts
Ref:	=1988AbaOB..65...18C
by	CHARGEISHVILI K.B.
	Byull. Abastumanskaya Astrofiz. Obs., 65, 18-None (1988)
	The catalogue of spectral and luminosity classes of 6037 stars in the direction of the galaxy anticenter.
o	Catalog: <AAO +DD NNN> N=6037
=E=	Catalogue in electronic form as <III/276/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AAS2009]
[AAS2009]	(Aoki+Arimoto+Sadakane+, 2009)
Write:	<<[AAS2009] S NN-NN>>
N:	8
Object:	* (SIMBAD class: Star)
Note:	Observations of the central regions of the Sextans dwarf spheroidal galaxy: INT WFC/WFI (optical photometry), UKIRT WFCAM (JHK observations), Subaru HDS (spectroscopy).
in source:	NAME Sextans Dwarf Galaxy
Ref:	=2009A&A...502..569A
by	AOKI W. , ARIMOTO N., SADAKANE K., TOLSTOY E., BATTAGLIA G., JABLONKA P., SHETRONE M., LETARTE B., IRWIN M., HILL V., FRANCOIS P., VENN K., PRIMAS F., HELMI A., KAUFER A., TAFELMEYER M., SZEIFERT T., BABUSIAUX C.
	Astron. Astrophys., 502, 569-578 (2009)
	Chemical composition of extremely metal-poor stars in the Sextans dwarf spheroidal galaxy.
o	Paragraph 4.1 Draco 119 is [BS61] 119 in Simbad, Sextans S49 is [SMT93] 49.
o	Table 1: <[AAS2009] S NN-NN> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AAT
AAT	(Anglo Australian Telescope)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: aat
aat	(AAT sample)
*****	Avoid the usage of aat, prefer [KGM99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AAT
AAT	(Anglo-Australian Telescope)
*****	Avoid the usage of AAT, prefer [RGC2002]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AAV2007]
[AAV2007]	(Ascenso+Alves+Vicente+, 2007) (Not yet in Simbad)
Write:	<<[AAV2007] JHHMMSS.s+DDMMSS>>
N:	2
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	NTT SOFI and VLT NACO observations of the cluster Trumpler 14. See also Cl* Trumpler 14 NACO and Cl* Trumpler 14 SOFI.
in source:	Cl Trumpler 14
Ref:	=2007A&A...476..199A
by	ASCENSO J. , ALVES J., VICENTE S., LAGO M.T.V.T.
	Astron. Astrophys., 476, 199-215 (2007)
	NTT and VLT diffraction limited imaging of Trumpler 14: revealing a massive core-halo cluster.
o	catalog NACO: <Cl* Trumpler 14 NACO NNN> (Nos 1-178). catalog SOFI: <Cl* Trumpler 14 SOFI NNNN> (Nos 1-4739). Text: <[AAV2007] JHHMMSS.s+DDMMSS> N=2.
=E=	Catalogue in electronic form as <J/A+A/476/199/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AAV2011]
[AAV2011]	(Ascaso+Aguerri+Varela+, 2011)
Write:	<<[AAV2011] JHHMMSS.sss+DDMMSS.ss>>
N:	20
Object:	Brightest Cluster Galaxy (SIMBAD class: BrightestCG = Brightest Galaxy in a Cluster (BCG))
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations of N=20 brightest cluster galaxies. The format is based on coordinates provided by the authors (priv. comm.).
Ref:	=2011ApJ...726...69A
by	ASCASO B. , AGUERRI J.A.L., VARELA J., CAVA A., BETTONI D., MOLES M., D'ONOFRIO M.
	Astrophys. J., 726, 69 (2011)
	Evolution of brightest cluster galaxy structural parameters in the last ~6 gyr: feedback processes versus merger events.
o	Table 2 (priv. comm.): <[AAV2011] JHHMMSS.sss+DDMMSS.ss> N=20.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AAVSO
AAVSO	(American Association of Variable Star Observers)
Write:	<<AAVSO HHMM+DDA>>
N:	5864
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	In the acronym format coordinates are 1900 coordinates. See AAVSO International Database (http://www.aavso.org).
Auth.:	AAVSO International Database
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AAZ2019]
[AAZ2019]	(Acebron+Alon+Zitrin+, 2019)
Write:	<<[AAZ2019] RX J0152.7-1357 N.N>> <<[AAZ2019] RX J0152.7-1357 cNN.N>>
N:	24+7
Object:	Grav. lensed image + Poss. Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=24 gravitationally lensed images and N=7 gravitationally lensed image candidates of N=10 multiply-imaged background sources by the galaxy cluster RX J0152.7-1357. Use of data from the RELICS Hubble Treasury program. See also [ACZ2018], [CAZ2018], [CSA2018], [PSC2018].
in source:	RX J0152.7-1357 = ClG J0152-1357
Ref:	=2019ApJ...874..132A
by	ACEBRON A. , ALON M., ZITRIN A., MAHLER G., COE D., SHARON K., CIBIRKA N., BRADAC M., TRENTI M., UMETSU K., ANDRADE-SANTOS F., AVILA R.J., BRADLEY L., CARRASCO D., CERNY C., CZAKON N.G., DAWSON W.A., FRYE B., HOAG A.T., HUANG K.-H., JOHNSON T.L., JONES C., KIKUCHIHARA S., LAM D., LIVERMORE R.C., LOVISARI L., MAINALI R., OESCH P.A., OGAZ S., OUCHI M., PAST M., PATERNO-MAHLER R., PETERSON A., RYAN R.E., SALMON B., SENDRA-SERVER I., STARK D.P., STRAIT V., TOFT S., VULCANI B.
	Astrophys. J., 874, 132-132 (2019)
	RELICS: high-resolution constraints on the inner mass distribution of the z = 0.83 merging cluster RXJ0152.7-1357 from strong lensing.
o	Fig. 1, Table 1: <[AAZ2019] RX J0152.7-1357 N.N> N=24 among (Nos 1.1-1.4 to 8.1-8.3), <[AAZ2019] RX J0152.7-1357 cNN.N> N=7 among (Nos c5.3, c9.1-9.3, c10.1-c10.3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AB
AB	(A. Braccesi)
Write:	<<AB NNN>>
N:	175
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Ref:	=1970A&A.....5..264B
by	BRACCESI A. , FORMIGGINI L., GANDOLFI E.
	Astron. Astrophys., 5, 264-279 (1970)
	Magnitudes, colours and coordinates of 175 ultraviolet excess objects in the field 13h, +36d.
o	(Erratum) Erratum A&A 23, p. 159-160 (1973)
o	Erratum gives the correct coordinates
o	<AB NNN> (Nos 1-175)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AB
AB	(Aspin+Barsony)
*****	Avoid the usage of AB, prefer [AB94]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ab
Ab	(Abell cl., bright)
*****	Avoid the usage of Ab, prefer [CSD91]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Ab
Ab	(Abastumni obs.)
*****	Avoid the usage of Ab, prefer KKO
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AB
AB	(Azzopardi+Breysacher)
*****	Avoid the usage of AB, prefer LMC AB
Origin	of the Acronym: L = Found in the literature
Details on Acronym: AB
AB	(Azzopardi+Breysacher)
*****	Avoid the usage of AB, prefer SMC AB
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [AB2002]
[AB2002]	(Altavilla+Benetti, 2002)
Write:	<<[AB2002] JHHMMSS.ss+DDMMSS.s>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxies of SN 2002CL, SN 2002CM, SN 2002CN.
Ref:	=2002IAUC.7885....2A
by	ALTAVILLA G. , BENETTI S.
	IAU Circ., 7885, 2-None (2002)
	Supernovae 2002cl, 2002cm, 2002cn, 2002co.
o	<[AB2002] JHHMMSS.ss+DDMMSS.s> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AB94]
[AB94]	(Aspin+Barsony, 1994)= (AB)
Write:	<<[AB94] NN>>
N:	51
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	NAME LkHA 101 Cluster
Ref:	=1994A&A...288..849A
by	ASPIN C. , BARSONY M.
	Astron. Astrophys., 288, 849-859 (1994)
	Near-IR imaging photometry of the J-K>4 sources in the Lk Hα 101 infrared cluster.
o	<[AB94] NN> N=51
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ABAO
ABAO	(Abastum. Astron. Obs.)
*****	Avoid the usage of ABAO, prefer [S78b]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [ABB2003]
[ABB2003]	(Alexander+Bauer+Brandt+, 2003)
Write:	<<[ABB2003] CDFN NNN>> <<[ABB2003] CDFN SNN>> <<[ABB2003] CDFS NNN>> <<[ABB2003] CDFS SNN>>
N:	503+79+326+42
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra survey of the Chandra Deep Field North (CDFN) and Chandra Deep Field South (CDFS). A Supplementary catalogue (format 'SNN') is added to the main catalogue in each field. See also [NLA2005].
in source:	NAME CDFN
in source:	NAME CDFS
Ref:	=2003AJ....126..539A
by	ALEXANDER D.M. , BAUER F.E., BRANDT W.N., SCHNEIDER D.P., HORNSCHEMEIER A.E., VIGNALI C., BARGER A.J., BROOS P.S., COWIE L.L., GARMIRE G.P., TOWNSLEY L.K., BAUTZ M.W., CHARTAS G., SARGENT W.L.W.
	Astron. J., 126, 539-574 (2003)
	The Chandra Deep Field North Survey. XIII. 2 Ms point-source catalogs.
o	Tables 3: <[ABB2003] CDFN NNN> (Nos 1-503). Tables 7: <[ABB2003] CDFN SNN> (Nos S1-S79). Tables A2: <[ABB2003] CDFS NNN> (Nos 1-326). Tables A3: <[ABB2003] CDFS SNN> (Nos S1-S42).
=E=	Catalogue in electronic form as J/AJ/126/539
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABB2006]
[ABB2006]	(AMI Collaboration+Barker+Biddulph+, 2006)
Write:	<<[ABB2006] A>>
N:	18
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=18 NVSS sources subtracted from Arcminute Microkelvin Imager (AMI) 15GHz observations of ACO 1914.
in source:	ACO 1914
Ref:	=2006MNRAS.369L...1A
by	AMI COLLABORATION , BARKER R., BIDDULPH P., BLY D., BOYSEN R., BROWN A., CLEMENTSON C., CROFTS M., CULVERHOUSE T., CZERES J., DACE R., D'ALESSANDRO R., DOHERTY P., DUFFETT-SMITH P., DUGGAN K., ELY J., FELVUS M., FLYNN W., GEISBUSCH J., GRAINGE K., GRAINGER W., HAMMET D., HILLS R., HOBSON M., HOLLER C., JILLEY R., JONES M.E., KANEKO T., KNEISSL R., LANCASTER K., LASENBY A., MARSHALL P., NEWTON F., NORRIS O., NORTHROP I., POOLEY G., QUY V., SAUNDERS R.D.E., SCAIFE A., SCHOFIELD J., SCOTT P., SHAW C., TAYLOR A.C., TITTERINGTON D., VELIC M., WALDRAM E., WEST S., WOOD B., YASSIN G., ZWART J.
	Mon. Not. R. Astron. Soc., 369, 1-4 (2006)
	High-significance Sunyaev-Zel'dovich measurement: Abell 1914 seen with the Arcminute Microkelvin Imager.
o	Table 1, Fig.4: <[ABB2006] A> (Nos A-R).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABB2011]
[ABB2011]	(Alexander+Bauer+Brandt+, 2011)
Write:	<<[ABB2011] JHHMMSS.ss+DDMMSS.s>>
N:	47
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Chandra X-ray observations of N=47 BzK galaxies in the Chandra Deep Field-South. See also [XLB2011].
in source:	NAME CDFS
Ref:	=2011ApJ...738...44A
by	ALEXANDER D.M. , BAUER F.E., BRANDT W.N., DADDI E., HICKOX R.C., LEHMER B.D., LUO B., XUE Y.Q., YOUNG M., COMASTRI A., DEL MORO A., FABIAN A.C., GILLI R., GOULDING A.D., MAINIERI V., MULLANEY J.R., PAOLILLO M., RAFFERTY D.A., SCHNEIDER D.P., SHEMMER O., VIGNALI C.
	Astrophys. J., 738, 44 (2011)
	X-ray spectral constraints for z ~ 2 massive galaxies: the identification of reflection-dominated active galactic nuclei.
o	Table 1: <[ABB2011] JHHMMSS.ss+DDMMSS.s> N=47.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABB2014]
[ABB2014]	(Anderson+Bania+Balser+, 2014)
Write:	<<[ABB2014] WISE GLLL.lll+BB.bbb>> <<[ABB2014] GLLL.lll+BB.bbb>>
N:	8399+133
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Catalog of N=8399 Galactic HII regions and HII region candidates from the all-sky WISE satellite. Format GLLL.lll+BB.bbb is for the sources that were not included in the Catalog. See also: http://astro.phys.wvu.edu/wise/
Ref:	=2014ApJS..212....1A
by	ANDERSON L.D. , BANIA T.M., BALSER D.S., CUNNINGHAM V., WENGER T.V., JOHNSTONE B.M., ARMENTROUT W.P.
	Astrophys. J., Suppl. Ser., 212, 1 (2014)
	The WISE catalog of Galactic H II regions.
o	Tables 2+5+6: <[ABB2014] WISE GLLL.lll+BB.bbb> N=8392. Table 3: <[ABB2014] GLLL.lll+BB.bbb> N=135.
=E=	Catalogue in electronic form as J/ApJS/212/1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABB2016]
[ABB2016]	(Ajello+Baldini+Barbiellini+, 2016) (Not yet in Simbad)
Write:	<<[ABB2016] SrcN>>
N:	4
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	N=4 background sources in the field of RCW 86. Use of Fermi LAT observations.
in source:	RCW 86
Ref:	=2016ApJ...819...98A
by	AJELLO M. , BALDINI L., BARBIELLINI G., BASTIERI D., BELLAZZINI R., BISSALDI E., BLOOM E.D., BONINO R., BOTTACINI E., BRANDT T.J., BREGEON J., BRUEL P., BUEHLER R., CALIANDRO G.A., CAMERON R.A., CARAGIULO M., CAVAZZUTI E., CHARLES E., CHEKHTMAN A., CIPRINI S., COHEN-TANUGI J., CONDON B., COSTANZA F., CUTINI S., D'AMMANDO F., DE PALMA F., DESIANTE R., DI LALLA N., DI MAURO M., DI VENERE L., DRELL P.S., DUBNER G., DUMORA D., DUVIDOVICH L., FAVUZZI C., FOCKE W.B., FUSCO P., GARGANO F., GASPARRINI D., GIACANI E., GIGLIETTO N., GLANZMAN T., GREEN D.A., GRENIER I.A., GUIRIEC S., HAYS E., HEWITT J.W., HILL A.B., HORAN D., JOGLER T., JOHANNESSON G., JUNG-RICHARDT I., KENSEI S., KUSS M., LARSSON S., LATRONICO L., LEMOINE-GOUMARD M., LI J., LI L., LONGO F., LOPARCO F., LOVELLETTE M.N., LUBRANO P., MAGILL J., MALDERA S., MANFREDA A., MAYER M., MAZZIOTTA M.N., McENERY J.E., MICHELSON P.F., MITTHUMSIRI W., MIZUNO T., MONZANI M.E., MORSELLI A., MOSKALENKO I.V., NEGRO M., NUSS E., ORIENTI M., ORLANDO E., ORMES J.F., PANEQUE D., PERKINS J.S., PESCE-ROLLINS M., PIRON F., PIVATO G., PORTER T.A., RAINO S., RANDO R., RAZZANO M., REIMER A., REIMER O., REPOSEUR T., SCHMID J., SCHULZ A., SGRO C., SIMONE D., SISKIND E.J., SPADA F., SPANDRE G., SPINELLI P., THAYER J.B., TIBALDO L., TORRES D.F., TOSTI G., TROJA E., UCHIYAMA Y., VIANELLO G., VINK J., WOOD K.S., YASSINE M.
	Astrophys. J., 819, 98 (2016)
	Deep morphological and spectral study of the SNR RCW 86 with Fermi-LAT.
o	Table 3: <[ABB2016] SrcN> (Nos Src1-Src4).
Details on Acronym: [ABB2020]
[ABB2020]	(Annibali+Beccari+Bellazzini+, 2020)
Write:	<<[ABB2020] SSH-UDG1>>
N:	1
Object:	Ultra-diffuse G (SIMBAD class: LowSurfBrghtG = Low Surface Brightness Galaxy)
Stat:	is completely incorporated in Simbad
Note:	LBT LBC observations of N=1 ultra diffuse galaxy (UDG) in the field of UGC 1281.
Ref:	=2020MNRAS.491.5101A
by	ANNIBALI F. , BECCARI G., BELLAZZINI M., TOSI M., CUSANO F., PARIS D., CIGNONI M., CIOTTI L., NIPOTI C., SACCHI E.
	Mon. Not. R. Astron. Soc., 491, 5101-5125 (2020)
	The Smallest Scale of Hierarchy survey (SSH) - I. Survey description.
o	Fig. 19, Table 2: <[ABB2020] SSH-UDG1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABC2001]
[ABC2001]	(Altavilla+Benetti+Cappellaro+, 2001)
Write:	<<[ABC2001] JHHMMSS.ss+DDMMSS.s>>
N:	6
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxies of SN 2001GE to SN 2001GJ.
Ref:	=2001IAUC.7762....1A
by	ALTAVILLA G. , BENETTI S., CAPPELLARO E., PASTORELLO A., RIELLO M., TURATTO M., ZAMPIERI L., CLOCCHIATTI A., CONTRERAS C., DANZIGER I.J., MAZZALI P., PATAT F.
	IAU Circ., 7762, 1-None (2001)
	Supernovae 2001ge, 2001gf, 2001gg, 2001gh, 2001gi, 2001gj.
o	<[ABC2001] JHHMMSS.ss+DDMMSS.s> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABC2002]
[ABC2002]	(Arp+Burbidge+Chu+, 2002)
Write:	<<[ABC2002] A>> <<[ABC2002] N>> <<[ABC2002] FN>>
N:	6+4+6
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	VLT observations. Fig.1, Table 1: probable QSOs, already cataloged, (Nos A-F) and (Nos 1-4). Fig.4, Table 2: Chain of 6 objects (Nos F1-F6) concentrated in a narrow X-ray filament.
in source:	NGC 3628
Ref:	=2002A&A...391..833A
by	ARP H. , BURBIDGE E.M., CHU Y., FLESCH E., PATAT F., RUPPRECHT G.
	Astron. Astrophys., 391, 833-840 (2002)
	NGC 3628: Ejection activity associated with quasars.
o	Fig.1, Table 1: <[ABC2002] A> (Nos A-F), <[ABC2002] N> (Nos 1-4). Fig.4, Table 2: <[ABC2002] AN> (Nos F1-F6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABC2005]
[ABC2005]	(Alexander+Bauer+Chapman+, 2005)
Write:	<<[ABC2005] JHHMMSS.ss+DDMMSS.s>>
N:	20
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	SCUBA-selected massive submillimeter-emitting galaxies (SMG). Combination of ultradeep X-ray observations (2Ms Chandra Deep Field North) and Deep Keck spectroscopy of SMG with radio counterparts.
in source:	NAME CDFN
Ref:	=2005ApJ...632..736A
by	ALEXANDER D.M. , BAUER F.E., CHAPMAN S.C., SMAIL I., BLAIN A.W., BRANDT W.N., IVISON R.J.
	Astrophys. J., 632, 736-750 (2005)
	The X-ray spectral properties of SCUBA galaxies.
o	Table 1: <[ABC2005] JHHMMSS.ss+DDMMSS.s> N=20.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABC2015]
[ABC2015]	(Armstrong+Brown+Chadwick+, 2015)
Write:	<<[ABC2015] JHHMM.m+DDMM>> <<[ABC2015] JHHMM.mm+DDMM>>
N:	13
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Detection of N=13 Fermi gamma-ray sources with the density-based clustering algorithm DBSCAN and not present in the 3FGL catalogue.
Ref:	=2015MNRAS.452.3159A
by	ARMSTRONG T. , BROWN A.M., CHADWICK P.M., NOLAN S.J.
	Mon. Not. R. Astron. Soc., 452, 3159-3166 (2015)
	The detection of Fermi AGN above 100 GeV using clustering analysis.
o	Table 2: <[ABC2015] JHHMM.mm+DDMM> N=10, <[ABC2015] JHHMM.m+DDMM> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABC89]
[ABC89]	(Aaronson+Blanco+Cook+, 1989)= ABCS = (Car) = (Cen) = (Cir) = (Cru) = (Pup) = (Ppx) = (Vel)
Write:	<<[ABC89] CCC NNNa>>
N:	44+46+76+117+100+67+40
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Note:	Northern C, see [ABC90] for Southern C
Ref:	=1989ApJS...70..637A
by	AARONSON M. , BLANCO V.M., COOK K.H., SCHECHTER P.L.
	Astrophys. J., Suppl. Ser., 70, 637-659 (1989)
	Southern Milky Way carbon stars: new candidates, JHK photometry and radial velocities.
o	Table 3B: cross-id Ppx 24 = CCS 1087 not 1987. Table 7A: CruS = CSS 820.
o	Table 2: <[ABC89] Pup NN> (Nos 1-44). Table 3: <[ABC89] Ppx NNa> (Nos 1-45), N=46. Table 4: <[ABC89] Vel NNa> (Nos 1-70), N=75. Table 5: <[ABC89] Car NNNa> (Nos 1-108), N=117. Table 6: <[ABC89] Cen NNN> (Nos 1-100). Table 7: <[ABC89] Cru NN> (Nos 1-67). Table 8: <[ABC89] Cir NNa> (Nos 1-39), N=40.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABC90]
[ABC90]	(Aaronson+Blanco+Cook+, 1990)= (caa) = (cab) = (cad) = (cep) = (cya) = (cyb) = (cyc) = (maa) = (vul)
Write:	<<[ABC90] aaa NN>> <<[ABC90] cyg wr1>>
N:	70+95+1+80+63+42+42+42+30+39
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Note:	Southern C, see [ABC89] for Northern C
Ref:	=1990ApJS...73..841A
by	AARONSON M. , BLANCO V.M., COOK K.H., OLSZEWSKI E.W., SCHECHTER P.L.
	Astrophys. J., Suppl. Ser., 73, 841-862 (1990)
	Northern Milky Way carbon star: new candidates, JHK photometry and radial velocities.
o	Table 2: <[ABC90] vul NN> (Nos 1-70). Table 3: <[ABC90] cya NN> (Nos 1-95). Table 4: <[ABC90] cyb NN> (Nos 1-80). Table 5: <[ABC90] cyc NN> (Nos 1-63). Table 6: <[ABC90] cep NN> (Nos 1-42). Table 7:<[ABC90] caa NN> (Nos 1-42). Table 8 : <[ABC90] cab NN> (Nos 1-42). Table 9 : <[ABC90] cad NN> (Nos 1-30). Table 10 : <[ABC90] maa NN> (Nos 1-46).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABC94]
[ABC94]	(Adanti+Battinelli+Capuzzo-Dolcetta+, 1994)
Write:	<<[ABC94] WW NN>> <<[ABC94] IF NN>>
N:	18+12+38
Object:	Clump (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Table 1: format 'NE NN' stands for North-East field, N=18 clumps Table 2: format 'SW NN' stands for South-West field, N=12 clumps Table 3: format 'IF NN' stands for Inner Field of NGC 2903, N=38 clumps
in source:	NGC 2903
Ref:	=1994A&AS..108..395A
by	ADANTI S. , BATTINELLI P., CAPUZZO-DOLCETTA R., HODGE P.W.
	Astron. Astrophys., Suppl. Ser., 108, 395-402 (1994)
	A new automatic identification technique for OB associations in unresolved galaxies.
o	Table 1: <[ABC94] NE NN> N=18. Table 2: <[ABC94] SW NN> N=12. Table 3: <[ABC94] IF NN> N=38
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABC99]
[ABC99]	(Abe+Bond+Carter+, 1999) (Not yet in Simbad)
Write:	<<[ABC99] N>>
N:	5
Object:	* (SIMBAD class: Star)
Note:	N=5 calibration stars.
Ref:	=1999AJ....118..261A
by	ABE F. , BOND I.A., CARTER B.S., DODD R.J., FUJIMOTO M., HEARNSHAW J.B., HONDA M., JUGAKU J., KABE S., KILMARTIN P.M., KORIBALSKI B.S., KOBAYASHI M., MASUDA K., MATSUBARA Y., MIYAMOTO M., MURAKI Y., NAKAMURA T., NANKIVELL G.R., NODA S., PENNYCOOK G.S., PIPE L.Z., RATTENBURY N.J., REID M., RUMSEY N.J., SAITO T., SATO H., SATO S., SEKIGUCHI M., SULLIVAN D.J., SUMI T., WATASE Y., YANAGISAWA T., YOCK P.C.M., YOSHIZAWA M.
	Astron. J., 118, 261-272 (1999)
	Observation of the halo of the edge-on galaxy IC 5249.
o	Fig.4: <[ABC99] N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ABCG
ABCG	(Abell, Cluster of G)
Write:	<<ABCG NNNN>>
N:	2712
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Revised and extended by ACO, 1989ApJS...70....1A
Ref:	=1958ApJS....3..211A
by	ABELL G.O.
	Astrophys. J., Suppl. Ser., 3, 211-288 (1958)
	The distribution of rich clusters of galaxies.
o	Table 6: <ABCG NNNN> (Nos 1-2712)
=E=	Catalogue in electronic form as VII/4
Details on Acronym: ABCG
ABCG	(Abell, Cluster of G)
====>	Equivalent to: ACO
Details on Acronym: ABCS
ABCS	(Aaronson+Blanco+Cook+Schechter)
====>	Equivalent to: [ABC89]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [ABD2005]
[ABD2005]	(Adami+Biviano+Durret+, 2005)
Write:	<<[ABD2005] GNN>>
N:	17
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	New multiwavelength analysis of the Coma cluster subclustering. See also [AIP2008].
in source:	Coma Cluster = ACO 1656
Ref:	=2005A&A...443...17A
by	ADAMI C. , BIVIANO A., DURRET F., MAZURE A.
	Astron. Astrophys., 443, 17-27 (2005)
	The build-up of the Coma cluster by infalling substructures.
o	Table1 and figures 3/4: read "NGC 4952" instead of "NGC 4852"
o	Table 2: <[ABD2005] GNN> (Nos G1-G17).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABD2011]
[ABD2011]	(Aspin+Beck+Davis+, 2011)
Write:	<<[ABD2011] GLLL.lll+BB.bbb>> <<[ABD2011] NN>>
N:	55
Object:	mm clump (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	CSO Bolocam observations of N=55 millimeter continuum clumps in the Braid Nebula.
in source:	NAME Braid Nebula
Ref:	=2011AJ....141..139A
by	ASPIN C. , BECK T.L., DAVIS C.J., FROEBRICH D., KHANZADYAN T., MAGAKIAN T.Yu., MORIARTY-SCHIEVEN G.H., MOVSESSIAN T.A., MITCHISON S., NIKOGOSSIAN E.G., PYO T.-S., SMITH M.D.
	Astron. J., 141, 139 (2011)
	CSO bolocam 1.1 mm continuum mapping of the braid nebula star formation region in Cygnus OB7.
o	Fig. 3, Tables 1+3: <[ABD2011] GLLL.lll+BB.bbb> N=55 = <[ABD2011] NN> (Nos 1-55). Table 2: <[MKM2003b] CNNW> (Nos CN1S, CN6N) added.
o	In table 2, 2MASS J20585089+5228254 is a probable misprint for 2MASS J20585089+5228227.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABD2014]
[ABD2014]	(Alarie+Bilodeau+Drissen, 2014)
Write:	<<[ABD2014] QSF NNa>>
N:	39
Object:	Clump (SIMBAD class: EmObj = Emission Object)
Note:	N=51 quasi-stationary flocculi (QSFs) in the field of Cassiopeia A. Observatoire du Mont Megantic SpIOMM spectroscopic observations. Use of HST archival data.
in source:	NAME Cas A
Ref:	=2014MNRAS.441.2996A
by	ALARIE A. , BILODEAU A., DRISSEN L.
	Mon. Not. R. Astron. Soc., 441, 2996-3008 (2014)
	A hyperspectral view of Cassiopeia A.
o	Fig. 2, Table 3: <[ABD2014] QSF NNa> (Nos 1-6, 7a-7c, 8a-8b, 9a-9b, 10-11, 12a-12b, 13-30, 31a-31c, 32-44).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABD2021]
[ABD2021]	(Aggarwal+Budavari+Deller+, 2021)
Write:	<<[ABD2021] JDDD.dddd+DD.dddd>>
N:	75
Object:	Poss. G (SIMBAD class: Galaxy_Candidate = Galaxy Candidate)
Note:	N=75 host galaxy candidates in the fields of 13 fast radio bursts (FRBs). Use of Gemini, VLT, and Keck data.
Ref:	=2021ApJ...911...95A
by	AGGARWAL K. , BUDAVARI T., DELLER A.T., EFTEKHARI T., JAMES C.W., PROCHASKA J.X., TENDULKAR S.P.
	Astrophys. J., 911, 95-95 (2021)
	Probabilistic association of transients to their hosts (PATH).
o	Table 5: <[ABD2021] JDDD.dddd+DD.dddd> N=75.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Abel
Abel	(Abell)
*****	Avoid the usage of Abel, prefer ACO
Details on Acronym: Abel
Abel	(Abell)
*****	Avoid the usage of Abel, prefer Palomar
Details on Acronym: Abel
Abel	(Abell)
*****	Avoid the usage of Abel, prefer A55
Details on Acronym: Abell
Abell	(Abell)
*****	Avoid the usage of Abell, prefer [A61]
Origin	of the Acronym: L (1978ApJ...219L..89M)
Details on Acronym: Abell
Abell	(Abell)
*****	Avoid the usage of Abell, prefer ACO
Details on Acronym: Abell
Abell	(Abell)
*****	Avoid the usage of Abell, prefer Palomar
Details on Acronym: Abell
Abell	(Abell)
*****	Avoid the usage of Abell, prefer A55
Details on Acronym: Abell
Abell	(Abell)
*****	Avoid the usage of Abell, prefer A66
Details on Acronym: Abetti
Abetti	(Discoverer's name)
*****	Avoid the usage of Abetti, prefer ABT
Details on Acronym: [ABF2008]
[ABF2008]	(Auger+Becker+Fassnacht, 2008)
Write:	<<[ABF2008] JHHMMSS.ss+DDMMSS.s>>
N:	14
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Keck I LRIS observations of the fields of N=14 radio galaxies. Use of SDSS data.
Ref:	=2008AJ....135.1311A
by	AUGER M.W. , BECKER R.H., FASSNACHT C.D.
	Astron. J., 135, 1311-1317 (2008)
	The environments of low- and high-luminosity radio galaxies at moderate redshifts.
o	Table 3: <[ABF2008] JHHMMSS.ss+DDMMSS.s> N=14.
o	Table 4: Except for the galaxy at 14 16 58.642 +12 03 30.708 not found in the SDSS, the group members are identified by their SDSS id in SIMBAD.
=E=	Catalogue in electronic form as J/AJ/135/1311
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABG2007]
[ABG2007]	(Audard+Briggs+Grosso+, 2007)
Write:	<<[ABG2007] NNNN>>
N:	2148
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton Optical Monitor Observations of the Taurus Molecular Cloud (TMC): XEST survey, Optical Monitor survey format 'FF-OM-NNN', also numbered 'NNNN'.
in source:	NAME TMC
Ref:	=2007A&A...468..379A
by	AUDARD M. , BRIGGS K.R., GROSSO N., GUEDEL M., SCELSI L., BOUVIER J., TELLESCHI A.
	Astron. Astrophys., 468, 379-390 (2007)
	The XMM-Newton Optical Monitor survey of the Taurus Molecular Cloud.
o	Catalog, col(1): <[ABG2007] NNNN> (Nos 1-2148) = Catalog, col(5): <XEST FF-OM-NNN> N=2148.
=E=	Catalogue in electronic form as J/A+A/468/379
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABG2011]
[ABG2011]	(Arce+Borkin+Goodman+, 2011)= (CPS)
Write:	<<[ABG2011] CPS NN>>
N:	12
Object:	Bubble (SIMBAD class: Bubble)
Stat:	is completely incorporated in Simbad
Note:	N=12 molecular shells in FCRAO 12CO(1-0) and 13CO(1-0) observations from the COMPLETE (COordinated Molecular Probe Line Extinction Thermal Emission) survey.
in source:	NAME Perseus Molecular Cloud
Ref:	=2011ApJ...742..105A
by	ARCE H.G. , BORKIN M.A., GOODMAN A.A., PINEDA J.E., BEAUMONT C.N.
	Astrophys. J., 742, 105 (2011)
	A bubbling nearby molecular cloud: complete shells in Perseus.
o	Figs 1-2, Tables 1-4: <[ABG2011] CPS NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABG85]
[ABG85]	(Aliakberov+Berlin+Gol'nev+, 1985)
Write:	<<[ABG85] NN>>
N:	98
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Observations with the Ratan-600 radio telescope.
Ref:	=1985AZh....62..482A
by	ALIAKBEROV K.D. , BERLIN A.B., GOL'NEV V.Y., LIPOVKA N.M., MINGALIEV M.G., NIZHEL'SKIJ N.A., SPANGENBERG E.E., SHARIPOVA L.M.
	Astron. Zh., 62, 482-490 (1985)
	High-resolution observations of compact H II regions.
o	Table I: <[ABG85] NN> (Nos 1-98)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ABGC
ABGC	(Abell, Galaxy Cluster)
*****	Avoid the usage of ABGC, prefer ACO
Details on Acronym: [ABH2000]
[ABH2000]	(Amadon+Blanc+Haissinski+, 2000)
Write:	<<[ABH2000] JHHMMSS.ss+DDMMSS.s>>
N:	6
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=6 galaxies, host of 6 SN.
Ref:	=2000IAUC.7384Q...1A
by	AMADON A. , BLANC G., HAISSINSKI J., RICH J., COUTURES C.
	IAU Circ., 7384, 1-None (2000)
	Supernovae 2000R, 2000S, 2000T, 2000U, 2000V, 2000W, 2000X.
o	<[ABH2000] JHHMMSS.ss+DDMMSS.s> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABH2020]
[ABH2020]	(Antwi-Danso+Barger+Haffner, 2020)
Write:	<<[ABH2020] a>>
N:	7
Object:	Cloudlet (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	Wisconsin H-Alpha Mapper (WHAM) observations of N=7 cloudlets in the Magellanic Leading Arm Extension.
in source:	NAME Magellanic Leading Arm Extension
Ref:	=2020ApJ...891..176A
by	ANTWI-DANSO J. , BARGER K.A., HAFFNER L.M.
	Astrophys. J., 891, 176-176 (2020)
	Hα distances to the Leading Arm of the Magellanic Stream.
o	Fig. 1, Table 1: <[ABH2020] a> (Nos a-g).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABH87]
[ABH87]	(Atteia+Barat+Hurley+, 1987)
Write:	<<[ABH87] NN>>
N:	84
Object:	(Gamma) (SIMBAD class: gammaBurst = Gamma-ray Burst)
Note:	Numbering of 84 gamma-ray bursts.
Ref:	=1987ApJS...64..305A
by	ATTEIA J.L. , BARAT C., HURLEY K., NIEL M., VEDRENNE G., EVANS W.D., FENIMORE E.E., KLEBESADEL R.W., LAROS J.G., CLINE T., DESAI U., TEEGARDEN B., ESTULIN I.V., ZENCHENKO V.M., KUZNETSOV A.V., KURT V.G.
	Astrophys. J., Suppl. Ser., 64, 305-382 (1987)
	A second catalog of γ-ray bursts : 1978-1980 localizations from the interplanetary network.
o	Table 1: <[ABH87] NN> (Nos 1-84) = <GRB YYMMDDA> N=84.
Details on Acronym: [ABJ2009]
[ABJ2009]	(Anderson+Bania+Jackson+, 2009)
Write:	<<[ABJ2009] ALLL.ll+BB.bba>>
N:	301
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	BU-FCRAO 13CO observations of a sample of N=301 Galactic HII regions. Source names identify the nebular type: ultra compat ("U"), compact ("C"), or diffuse ("D").
Ref:	=2009ApJS..181..255A
by	ANDERSON L.D. , BANIA T.M., JACKSON J.M., CLEMENS D.P., HEYER M., SIMON R., SHAH R.Y., RATHBORNE J.M.
	Astrophys. J., Suppl. Ser., 181, 255-271 (2009)
	The molecular properties of galactic H II regions.
o	Tables 2-3: <[ABJ2009] ALLL.ll+BB.bba> N=301.
Ref:	=2009ApJ...690..706A
by	ANDERSON L.D. , BANIA T.M.
	Astrophys. J., 690, 706-719 (2009)
	Resolution of the distance ambiguity for galactic H II regions.
=E=	Catalogue in electronic form as J/ApJS/181/255
=E=	Catalogue in electronic form as J/ApJ/690/706
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABL2013]
[ABL2013]	(Andrews+Barrientos+Lopez+, 2013)
Write:	<<[ABL2013] JHHMMSS.ss+DDMMSS.ss>>
N:	437
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Gemini South GMOS observations of N=440 galaxies in the fields of nine QSOs.
Ref:	=2013ApJ...774...40A
by	ANDREWS H. , BARRIENTOS L.F., LOPEZ S., LIRA P., PADILLA N., GILBANK D.G., LACERNA I., MAUREIRA M.J., ELLINGSON E., GLADDERS M.D., YEE H.K.C.
	Astrophys. J., 774, 40 (2013)
	Galaxy clusters in the line of sight to background quasars. III. Multi-object spectroscopy.
o	Tables 3-11: <[ABL2013] JHHMMSS.ss+DDMMSS.ss> N=437.
=E=	Catalogue in electronic form as J/ApJ/774/40
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABM2007]
[ABM2007]	(Arias+Barba+Morrell, 2007)
Write:	<<[ABM2007] NN>>
N:	46
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	6.5m Magellan I telescope Boller & Chivens spectrograph observations of M 8.
in source:	M 8 = Lagoon Nebula
Ref:	=2007MNRAS.374.1253A
by	ARIAS J.I. , BARBA R.H., MORRELL N.I.
	Mon. Not. R. Astron. Soc., 374, 1253-1263 (2007)
	Pre-main-sequence stars in the Lagoon Nebula (M8).
o	Table 1: <[ABM2007] NN> (Nos 1-46).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABM2013]
[ABM2013]	(Aguirre+Baker+Menanteau+, 2013) (Not yet in Simbad)
Write:	<<[ABM2013] SMM J02399-0136 L1sb>>
N:	1
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST NICMOS and WFC3 observations of N=1 starburst component in the field of [ISL98] L1.
in source:	[ISL98] L1
Ref:	=2013ApJ...768..164A
by	AGUIRRE P. , BAKER A.J., MENANTEAU F., LUTZ D., TACCONI L.J.
	Astrophys. J., 768, 164 (2013)
	High-resolution near-infrared imaging of submillimeter galaxies.
o	Fig. 1, Paragr. 4.2.1: <[ABM2013] SMM J02399-0136 L1sb> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ABMMR
ABMMR	(Arias+Barba+Maiz-Apellaniz+Morrell+Rubio)
Write:	<<ABMMR NNN>>
N:	762
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Images of the Hourglass region obtained using the near-IR camera IRCAM at Las Campanas Observatory, complemented with archival HST WFPC2 images and ESO NTT EMMI spectra.
in source:	M 8:Hourglass Cluster = Hourglass Cluster
Ref:	=2006MNRAS.366..739A
by	ARIAS J.I. , BARBA R.H., MAIZ-APELLANIZ J., MORRELL N.I., RUBIO M.
	Mon. Not. R. Astron. Soc., 366, 739-757 (2006)
	The infrared Hourglass cluster in M8.
o	Table 4: <ABMMR NNN> (Nos 1-762).
=E=	Catalogue in electronic form as J/MNRAS/366/739
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ABP2001]
[ABP2001]	(Altavilla+Benetti+Pastorello+, 2001)
Write:	<<[ABP2001] JHHMMSS.ss+DDMMSS.s>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxies of SN 2001IO and SN 2001IP.
Ref:	=2001IAUC.7780....1A
by	ALTAVILLA G. , BENETTI S., PASTORELLO A., RIELLO M., TURATTO M., ZAMPIERI L., CAPPELLARO E., CLOCCHIATTI A., CONTRERAS C., DANZIGER I.J., MAZZALI P., PATAT F.
	IAU Circ., 7780, 1-None (2001)
	Supernovae 2001io and 2001ip.
o	<[ABP2001] JHHMMSS.ss+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABP2002]
[ABP2002]	(Altavilla+Benetti+Pastorello+, 2002)
Write:	<<[ABP2002] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of SN 2002DU.
Ref:	=2002IAUC.7929....2A
by	ALTAVILLA G. , BENETTI S., PASTORELLO A., RIELLO M., TURATTO M., ZAMPIERI L., CAPPELLARO E., CLOCCHIATTI A., CONTRERAS C., DANZIGER I.J., MAZZALI P., PATAT F.
	IAU Circ., 7929, 2-None (2002)
	Supernova 2002du.
o	<[ABP2002] JHHMMSS.ss+DDMMSS.s> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABP2009]
[ABP2009]	(Aspin+Beck+Pyo+, 2009)
Write:	<<[ABP2009] Braid star>> <<[ABP2009] HH627-STAR>> <<[ABP2009] IRAS NNW>>
N:	1+1+3
Object:	* (SIMBAD class: Star)
Note:	UKIRT WFCAM photometry and UIST spectroscopy of stars in the Braid Nebula region. See also [MKM2003b].
Ref:	=2009AJ....137..431A
by	ASPIN C. , BECK T.L., PYO T.-S., DAVIS C.J., SCHIEVEN G.M., KHANZADYAN T., MAGAKIAN T.Y., MOVSESSIAN T.A., NIKOGOSSIAN E.G., MITCHISON S., SMITH M.D.
	Astron. J., 137, 431-449 (2009)
	Near-IR spectroscopy of young stars in the Braid Nebula star formation region in Cygnus OB7.
o	Table 1: <[MKM2003b] AANW> (Nos CN6 to CN8, CN3N, CN3S) added. Table 1: <[ABP2009] Braid star> N=1, <[ABP2009] HH627-STAR> N=1, <[ABP2009] IRAS NNW> (Nos 14, 15N, 15S).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABP2017]
[ABP2017]	(Adam+Bartalucci+Pratt+, 2017)
Write:	<<[ABP2017] SMGNN>>
N:	11
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	IRAM 30m telescope NIKA observations of N=11 submillimeter point sources in the field of the galaxy cluster MCS J0717.5+3745.
in source:	ClG J0717+3745 = MCS J0717.5+3745
Ref:	=2017A&A...598A.115A
by	ADAM R. , BARTALUCCI I., PRATT G.W., ADE P., ANDRE P., ARNAUD M., BEELEN A., BENOIT A., BIDEAUD A., BILLOT N., BOURDIN H., BOURRION O., CALVO M., CATALANO A., COIFFARD G., COMIS B., D'ADDABBO A., DE PETRIS M., DEMOCLES J., DESERT F.-X., DOYLE S., EGAMI E., FERRARI C., GOUPY J., KRAMER C., LAGACHE G., LECLERCQ S., MACIAS-PEREZ J.-F., MAUROGORDATO S., MAUSKOPF P., MAYET F., MONFARDINI A., MROCZKOWSKI T., PAJOT F., PASCALE E., PEROTTO L., PISANO G., POINTECOUTEAU E., PONTHIEU N., REVERET V., RITACCO A., RODRIGUEZ L., ROMERO C., RUPPIN F., SCHUSTER K., SIEVERS A., TRIQUENEAUX S., TUCKER C., ZEMCOV M., ZYLKA R.
	Astron. Astrophys., 598A, 115-115 (2017)
	Mapping the kinetic Sunyaev-Zel'dovich effect toward MACS J0717.5+3745 with NIKA.
o	Table 4: <[ABP2017] SMGNN> (Nos SMG01-SMG11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ABS
ABS	(Azzopardi+Breysacher, SMC)
*****	Avoid the usage of ABS, prefer SMC AB
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [ABS2005]
[ABS2005]	(Almoznino+Brosch+Shara+, 2005)
Write:	<<[ABS2005] NNNNNN>>
N:	127
Object:	* (SIMBAD class: Star)
Note:	CTIO observations of stars to search optical counterparts of Far-UV [BSM99] objects among about 830000 stars in the LMC.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2005MNRAS.357..645A
by	ALMOZNINO E. , BROSCH N., SHARA M., ZUREK D.
	Mon. Not. R. Astron. Soc., 357, 645-655 (2005)
	The deepest Hubble Space Telescope far-ultraviolet observations in the Large Magellanic Cloud.
o	P. 646 : SNR N49 = LHA 120-N 49, N132D = LHA 120-N 132D.
o	Table 2, col(9): <[ABS2005] NNNNNN> N=127 among 830000.
=E=	Catalogue in electronic form as J/MNRAS/357/645
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABS98]
[ABS98]	(Andreuzzi+Bardelli+Scaramella+, 1998)
Write:	<<[ABS98] JHHMMSS.s+DDMMSS.s>>
N:	180
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Survey of galaxies in an area between the 2 ClG ACO 548 and ACO 3367. The area is divided into 6 fields (Tables 2 to 7)
Ref:	=1998A&A...337...17A
by	ANDREUZZI G. , BARDELLI S., SCARAMELLA R., ZUCCA E.
	Astron. Astrophys., 337, 17-24 (1998)
	A redshift survey between the clusters of galaxies A 548 and A 3367.
o	Tables 2-7: <[ABS98] JHHMMSS.s-DDMMSS.s> N=180.
=E=	Catalogue in electronic form as J/A+A/337/17
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ABT
ABT	(Discoverer's name)= (Abetti)
Write:	<<** ABT NN>>
N:	23
Object:	(SIMBAD class: = Double or Multiple Star)
Details on Acronym: [ABT94]
[ABT94]	(Ajhar+Blakeslee+Tonry, 1994)
Write:	<<[ABT94] NGC NNNN NN>>
N:	357
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Note:	Table 3: format 'NGC 3379 NN', N=60 Table 4: format 'NGC 4365 NN', N=41 Table 5: format 'NGC 4374 NN', N=41 Table 6: format 'NGC 4406 NN', N=41 Table 7: format 'NGC 4458 NN', N=29 Table 8: format 'NGC 4468 NN', N=21 Table 9: format 'NGC 4472 NN', N=41 Table 10: format 'NGC 4489 NN', N=16 Table 11: format 'NGC 4552 NN', N=41 Table 12: format 'NGC 4578 NN', N=26
in source:	NGC 3379
in source:	NGC 4365
in source:	NGC 4374 = M 84
in source:	NGC 4406 = M 86
in source:	NGC 4458
in source:	NGC 4468
in source:	NGC 4472 = M 49
in source:	NGC 4489
in source:	NGC 4552
in source:	NGC 4578
Ref:	=1994AJ....108.2087A
by	AJHAR E.A. , BLAKESLEE J.P., TONRY J.L.
	Astron. J., 108, 2087-2101 (1994)
	VRI photometry of globular clusters in Virgo and Leo ellipticals.
o	Tables 3 to 12: <[ABT94] NGC NNNN NN> N=60+41+41+41+29+21+41+16+41+26
=E=	Catalogue in electronic form as J/AJ/108/2087
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ABW-A
ABW-A	(Azzopardi, Breysacher, Westerlund, field A)
Write:	<<ABW-A NNN>>
N:	261
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Note:	Circular fields of 0.78 sq.deg , spectral range 4350-5300Å, grism. Table II: 261 stars identified as carbon stars among (Nos 1-323) in field A centered at alf(1975) = 00h50m, Dec(1975) = -73deg 30m
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1986A&AS...65...79W
by	WESTERLUND B.E. , AZZOPARDI M., BREYSACHER J.
	Astron. Astrophys., Suppl. Ser., 65, 79-95 (1986)
	Carbon stars in the Small Magellanic Cloud. I. The survey technique and results for two fields.
o	Table II: <ABW-A NNN> N=261 among (Nos 1-323). Table III: <ABW-B NNN> N=121 among (Nos 1-137).
Details on Acronym: ABW-B
ABW-B	(Azzopardi, Breysacher, Westerlund, field B)
Write:	<<ABW-B NNN>>
N:	121
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Note:	Circular fields of 0.78 sq.deg , spectral range 4350-5300Å, grism. Table III: 121 stars identified as carbon stars among (Nos 1-137). in field B centered at alf(1975) =01h02m, Dec(1975) = -72deg 15m
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1986A&AS...65...79W
by	WESTERLUND B.E. , AZZOPARDI M., BREYSACHER J.
	Astron. Astrophys., Suppl. Ser., 65, 79-95 (1986)
	Carbon stars in the Small Magellanic Cloud. I. The survey technique and results for two fields.
o	Table II: <ABW-A NNN> N=261 among (Nos 1-323). Table III: <ABW-B NNN> N=121 among (Nos 1-137).
Details on Acronym: [ABW2001]
[ABW2001]	(Augusto+Browne+Wilkinson+, 2001)
Write:	<<[ABW2001] B2114+022 A>> <<[ABW2001] GN>>
N:	4+2
Object:	Component + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	VLA, MERLIN, and HST maps of JVAS 2114+022 reveal 4 compact components (Nos A-D) and 2 galaxies (Nos G1-G2), G1 being the main lensing G.
Ref:	=2001MNRAS.326.1007A
by	AUGUSTO P. , BROWNE I.W.A., WILKINSON P.N., JACKSON N.J., FASSNACHT C.D., MUXLOW T.W.B., HJORTH J., JAUNSEN A.O., KOOPMANS L.V., PATNAIK A.R., TAYLOR G.B.
	Mon. Not. R. Astron. Soc., 326, 1007-1014 (2001)
	B2114+022: a distant radio source gravitationally lensed by a starburst galaxy.
o	Table 4, Figs1,2: <[ABW2001] B2114+022 A> (Nos A-D), <[ABW2001] GN> (Nos G1-G2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ABW75]
[ABW75]	(Arp+Baldwin+Wampler, 1975)
Write:	<<[ABW75] NGC 5682 QSO>> <<[ABW75] IC 1417 QSO>>
N:	2
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Ref:	=1975ApJ...198L...3A
by	ARP H. , BALDWIN J.A., WAMPLER E.J.
	Astrophys. J., 198, 3-5 (1975)
	Two new quasars near galaxies.
o	[ABW75] NGC 5682 QSO = NGC 5682 BSO 1 in Veron. [ABW75] IC 1417 QSO = [A81b] NGC 7171 BSO 1
o	<[ABW75] NGC 5682 QSO>, <[ABW75] IC 1417 QSO>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ABWR
ABWR	(Azzopardi+Breysacher, WR*)
*****	Avoid the usage of ABWR, prefer LMC AB
Origin	of the Acronym: L = Found in the literature
Details on Acronym: ABWR
ABWR	(Azzopardi+Breysacher, WR*)
*****	Avoid the usage of ABWR, prefer SMC AB
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: AC
AC	(A. Clark)
Write:	<<** AC NN>>
N:	20
Object:	(SIMBAD class: = Double or Multiple Star)
Auth.:	CLARK A.
Details on Acronym: AC
AC	(Astrographic Catalog)= (A) = (Gr) = (Grw)
Write:	<<AC +DD NNNNN>> <<AC +DD NNNNN A>> <<AC +DD NNNN-NNN>>
Object:	* (SIMBAD class: Star)
Note:	Description of,and explanations about astrographic catalogues and catalogues of accurate positions of stars. See also the catalogues of catalogues by Sevarlic et al. also quoted in the introduction. See also AC2000
Ref:	=1974asp...B......0E
by	EICHHORN H.
	Astronomy of star positions, 0-None (1974)
	A critical investigation of star catalogues, the methods of their construction and their purpose.
=E=	Catalogue in electronic form as I/154
=E=	Catalogue in electronic form as I/21
=E=	Catalogue in electronic form as I/22
Details on Acronym: AC
AC	(Abell+Corwin)
*****	Avoid the usage of AC, prefer ACCG
Origin	of the Acronym: L = Found in the literature
Details on Acronym: AC
AC	(Abell, Cluster of G)
*****	Avoid the usage of AC, prefer ACO
Details on Acronym: AC
AC	(AntiCenter cloud complex)
Note:	HVC Complex AC
*****	Avoid the usage of AC, prefer [H68]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AC2000
AC2000	(Astrographic Catalogue, 2000)
Write:	<<AC2000 NNNNNNN>>
N:	4621751
Object:	* (SIMBAD class: Star)
Note:	'The AC2000: the Astrographic Catalogue on the Hipparcos System'. The United States Naval Observatory has completed the reductions of the Astrographic Catalogue data AC to a consistent system. The resulting catalog, called AC 2000, contains 4621836 stars covering the entire sky, at an average epoch of 1907. The positions are on the Hipparcos reference frame (J2000.0) at the epochs of observation. The catalogue is revised (1998AJ....115.1212U) and contains 4621751 stars.
Ref:	=1998AJ....115.1212U
by	URBAN S.E. , CORBIN T.E., WYCOFF G.L., MARTIN J.C., JACKSON E.S., ZACHARIAS M.I., HALL D.M.
	Astron. J., 115, 1212-1224 (1998)
	The AC 2000: the astrographic catalogue on the system defined by the Hipparcos catalogue.
o	<AC2000 NNNNNNN> N=4621751.
=E=	Catalogue in electronic form as I/275
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AC2000b]
[AC2000b]	(Abt+Corbally, 2000)= (Trap)
Write:	<<[AC2000b] Trap NNN>> <<[AC2000b] Trap NNN NN>>
N:	265+1592
Object:	Group of * (SIMBAD class: ** = Double or Multiple Star)
Note:	N=265 Trapezium systems (physical systems of 3 or more stars) format 'Trap NNN'. N=1592 * in all the systems, format 'Trap NNN NN'. The systems are selected from an unpublished catalogue by Allen, Tapia and Parrao (see 1977RMxAA...3..119A).
Ref:	=2000ApJ...541..841A
by	ABT H.A. , CORBALLY C.J.
	Astrophys. J., 541, 841-848 (2000)
	The maximum age of Trapezium systems.
o	Table 3a: <[AC2000b] Trap NNN> N=265 among (Nos 1-966). Table 3b: <[AC2000b] Trap NNN NN> N=1592.
=E=	Catalogue in electronic form as J/ApJ/541/841
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AC95]
[AC95]	(Alves+Cook, 1995)
Write:	<<[AC95] VN>>
N:	9
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	(Nos V1-V4) are Cepheids, (Nos V5-V9) are Miras
in source:	M 101 = NGC 5457
Ref:	=1995AJ....110..192A
by	ALVES D.R. , COOK K.H.
	Astron. J., 110, 192-198 (1995)
	Ground-based discovery of Cepheids and Miras in M 101.
o	Table 2: <[AC95] VN> (Nos V1 to V9)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ACA2003]
[ACA2003]	(Alexander+Casali+Andre+, 2003)
Write:	<<[ACA2003] R CrA N>> <<[ACA2003] rho Oph A N>> <<[ACA2003] rho Oph E N>> <<[ACA2003] Ser A N>> <<[ACA2003] Ser B NN>> <<[ACA2003] Cha I N>>
N:	7+4+6+7+13+6
Object:	(Mid IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	ISOCAM Mid IR observations. Spectroscopy of YSOs and their environment in 4 star formation regions: R CrA, rho Oph, Serpens and Cha I.
in source:	NAME R CrA Cloud
in source:	NAME rho Oph Cloud
in source:	NAME Serpens Cloud
in source:	NAME Cha I
Ref:	=2003A&A...401..613A
by	ALEXANDER R.D. , CASALI M.M., ANDRE P., PERSI P., EIROA C.
	Astron. Astrophys., 401, 613-624 (2003)
	ISOCAM-CVF spectroscopy of the circumstellar environment of young stellar objects.
o	Table 1: <[ACA2003] R CrA N> (Nos 1-7), <[ACA2003] ρ Oph A N> (Nos 1-4), <[ACA2003] ρ Oph E N> (Nos 1-6), <[ACA2003] Ser A N> (Nos 1-7), <[ACA2003] Ser B NN> (Nos 1-13), <[ACA2003] Cha I N> (Nos 1-6).
=E=	Catalogue in electronic form as J/A+A/401/613
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ACB2016]
[ACB2016]	(Adam+Comis+Bartalucci+, 2016)
Write:	<<[ACB2016] SMGNN>>
N:	17
Object:	smm G (SIMBAD class: Galaxy)
Note:	IRAM 30m telescope NIKA observations of N=17 Herschel submillimeter galaxies. Use of Herschel SPIRE and PACS data, part of the Herschel Lensing Survey (HLS).
in source:	MCS J1423.8+2404
Ref:	=2016A&A...586A.122A
by	ADAM R. , COMIS B., BARTALUCCI I., ADANE A., ADE P., ANDRE P., ARNAUD M., BEELEN A., BELIER B., BENOIT A., BIDEAUD A., BILLOT N., BOURRION O., CALVO M., CATALANO A., COIFFARD G., D'ADDABBO A., DESERT F.-X., DOYLE S., GOUPY J., HASNOUN B., HERMELO I., KRAMER C., LAGACHE G., LECLERCQ S., MACIAS-PEREZ J.-F., MARTINO J., MAUSKOPF P., MAYET F., MONFARDINI A., PAJOT F., PASCALE E., PEROTTO L., POINTECOUTEAU E., PONTHIEU N., PRATT G.W., REVERET V., RITACCO A., RODRIGUEZ L., SAVINI G., SCHUSTER K., SIEVERS A., TRIQUENEAUX S., TUCKER C., ZYLKA R.
	Astron. Astrophys., 586A, 122-122 (2016)
	High angular resolution Sunyaev-Zel'dovich observations of MACS J1423.8+2404 with NIKA: Multiwavelength analysis.
o	Table 3: <[ACB2016] SMGNN> (Nos SMG01-SMG17).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ACCG
ACCG	(Abell+Corwin, Cluster of G)= (AC)
Write:	<<ACCG NNN>>
N:	30
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	Unpublished, (Nos 101-130)
Auth.:	ABELL G.O.+
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [ACD2011]
[ACD2011]	(Alberts+Calzetti+Dong+, 2011)
Write:	<<[ACD2011] NGC NNNN NN>>
N:	229
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Note:	GALEX and Spitzer IRAC observations of N=229 star-forming associations in the extended ultraviolet disks of five nearby spiral galaxies.
in source:	NGC 628 = M 74
in source:	NGC 2090
in source:	NGC 2841
in source:	NGC 3621
in source:	NGC 5055 = M 63
Ref:	=2011ApJ...731...28A
by	ALBERTS S. , CALZETTI D., DONG H., JOHNSON L.C., DALE D.A., BIANCHI L., CHANDAR R., KENNICUTT R.C., MEURER G.R., REGAN M., THILKER D.
	Astrophys. J., 731, 28 (2011)
	The evolution of stellar populations in the outer disks of spiral galaxies.
o	Tables 4-5: <[ACD2011] NGC NNNN NN> (Nos NGC 0628 1 to 32, NGC 2090 1 to 47, NGC 2841 1 to 75, NGC 3621 1 to 58, NGC 5055 1 to 17).
=E=	Catalogue in electronic form as <J/ApJ/731/28/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ACD2015]
[ACD2015]	(Adami+Cypriano+Durret+, 2015)
Write:	<<[ACD2015] D3-43 NN>> <<[ACD2015] D3-6 NN>> <<[ACD2015] D3-43 S3>>
N:	15+26+1
Object:	* + G + ClG (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Gemini GMOS spectroscopic observations of N=23+14 galaxies in two galaxy structures D3-43 and D3-3 within the CFHTLS Deep 3 field. Use of archival X-ray Chandra data.
in source:	[ADB2010] D3-43
in source:	[ADB2010] D3-6
Ref:	=2015A&A...575A..69A
by	ADAMI C. , CYPRIANO E.S., DURRET F., LE BRUN V., LIMA NETO G.B., MARTINET N., PEREZ F., ROUZE B., SODRE L.Jr
	Astron. Astrophys., 575A, 69-69 (2015)
	Two spectroscopically confirmed galaxy structures at z = 0.61 and 0.74 in the CFHTLS Deep 3 field.
o	Table 1: <[ACD2015] D3-43 NN> (Nos 1-15). Table 2: <[ACD2015] D3-6 NN> (Nos 1-26). Table 4: <[ACD2015] D3-43 S3>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ACE99]
[ACE99]	(Aussel+Cesarsky+Elbaz+, 1999)
Write:	<<[ACE99] HDF PMN.NN>> <<[ACE99] HDF PSN.NNa>>
N:	49+51
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	ISO CAM observations In the format 'PM' stands for PRETI Main, 'PS' for 'PRETI Supplementary, the first digit 'N' stands for the number of the LW field, 'NN' the numbering of the source, 'NNa' being neighbour of the source with same 'NN'. See also ISOHDF, [GOS97], [DPC99]
in source:	NAME HDFN
Ref:	=1999A&A...342..313A
by	AUSSEL H. , CESARSKY C.J., ELBAZ D., STARCK J.L.
	Astron. Astrophys., 342, 313-336 (1999)
	ISOCAM observations of the Hubble Deep Field reduced with the PRETI method.
o	Table 6, HDF_{PS3}40 misprint for PM3_40 (in SIMBAD : [ACE99] HDF PM3.40 )
o	Table 3: <[ACE99] HDF PMN.NN> N=49, = <ISOHDF JHHMMSS.s+DDMMSS> N=49. Table 4: <[ACE99] HDF PSN.NNa> N=51 = <ISOHDF JHHMMSS.s+DDMMSS> N=51.
=E=	Catalogue in electronic form as J/A+A/342/313
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ACF2018]
[ACF2018]	(Arrigoni Battaia+Chen+Fumagalli+, 2018) (Not yet in Simbad)
Write:	<<[ACF2018] SMM JHHMMSS.s+DDMMSS>> <<[ACF2018] MAM-850.NN>> <<[ACF2018] MAM-450.NN>>
N:	41+27+14
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	JCMT SCUBA-2 850µm and 450µm observations of N=27+14 sources around the MAMMOTH-1 nebula.
in source:	NAME MAMMOTH-1
Ref:	=2018A&A...620A.202A
by	ARRIGONI BATTAIA F. , CHEN C.-C., FUMAGALLI M., CAI Z., CALISTRO RIVERA G., XU J., SMAIL I., PROCHASKA J.X., YANG Y., DE BREUCK C.
	Astron. Astrophys., 620A, 202-202 (2018)
	Overdensity of submillimeter galaxies around the z ~= 2.3 MAMMOTH-1 nebula. The environment and powering of an enormous Lyman-α nebula.
o	Table 2, col(1): <[ACF2018] SMM JHHMMSS.s+DDMMSS> N=27 = :Table 2, col(2): <[ACF2018] MAM-850.NN> (Nos 850.1-850.27). Table 3, col(1): <[ACF2018] SMM JHHMMSS.s+DDMMSS> N=14 = Table 3, col(2): <[ACF2018] MAM-450.N> (Nos 450.1-450.14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ACF2023]
[ACF2023]	(Adams+Conselice+Ferreira+, 2023)
Write:	<<[ACF2023] NNNNN>>
N:	7
Object:	Poss. G (SIMBAD class: Galaxy_Candidate = Galaxy Candidate)
Note:	N=7 galaxy candidates in the JWST NIRCam parallel field of the SMACS J0723.3-7327 cluster. Use of JWST archival NIRCam data.
Ref:	=2023MNRAS.518.4755A
by	ADAMS N.J. , CONSELICE C.J., FERREIRA L., AUSTIN D., TRUSSLER J.A.A., JUODZBALIS I., WILKINS S.M., CARUANA J., DAYAL P., VERMA A., VIJAYAN A.P.
	Mon. Not. R. Astron. Soc., 518, 4755-4766 (2023)
	Discovery and properties of ultra-high redshift galaxies (9 < z < 12) in the JWST* ERO SMACS 0723 Field.*
o	F200DB-098 is a misprint for F200DA-098.
o	Table 3: <[ACF2023] NNNNN> N=7 among (Nos 1514-10234).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: ACG
ACG	(Arp, Compact G)= (CG)
Write:	<<ACG HHMM+DD>>
N:	2
Object:	Compact G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=2, ACG 1116+51 and ACG 1124+54 Rounded, not truncated coordinates
Ref:	=1975ApJ...197..291A
by	ARP H. , O'CONNELL R.W.
	Astrophys. J., 197, 291-296 (1975)
	Properties of two blue compact galaxies.
o	<ACG HHMM+DD> N=2.
Details on Acronym: [ACG2002]
[ACG2002]	(Appleton+Charmandaris+Gao+, 2002)
Write:	<<[ACG2002] NN>> <<[ACG2002] MIR Knot>>
N:	2+1
Object:	G + (IR) (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ISO and BIMA observations of NGC 985. NGC 985 contains 2 closely spaced nuclei, N1 and N2. A bright Middle-IR Knot is observed by ISO. See also [AM93].
in source:	NGC 985
Ref:	=2002ApJ...566..682A
by	APPLETON P.N. , CHARMANDARIS V., GAO Y., COMBES F., GHIGO F., HORELLOU C., MIRABEL I.F.
	Astrophys. J., 566, 682-698 (2002)
	Mid-infrared and CO observations of the Infrared/X-ray luminous Seyfert 1 galaxy NGC 985: the making or breaking of a ULIRG.
o	Sources p. 684 : 0238+166, 0339-017 with 2000 coord. are RORF 0235+164 and RORF 0336-019
o	Fig.2: <[ACG2002] AN> (Nos N1, N2). Table 1: <[ACG2002] MIR Knot> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ACG2003]
[ACG2003]	(Appleton+Charmandaris+Gao+, 2003) (Not yet in Simbad)
Write:	<<[ACG2003] A>> <<[ACG2003] A'>>
N:	4+1
Object:	HI Clump (SIMBAD class: HI = HI (21cm) Source)
Note:	HI observations of the galaxy NGC 1144. N=4 clumps (Nos A-D), and A' component of A. See also [GSD97].
in source:	NGC 1144
Ref:	=2003ApJ...586..112A
by	APPLETON P.N. , CHARMANDARIS V., GAO Y., JARRETT T., BRANSFORD M.A.
	Astrophys. J., 586, 112-122 (2003)
	Azimuthal and kinematic segregation of neutral and molecular gas in Arp 118: the yin-yang galaxy NGC 1144.
o	Text, Fig.2: <[ACG2003] A> (Nos A-D), <[ACG2003] A'> (No. A').
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ACG2016]
[ACG2016]	(Ainsworth+Coughlan+Green+, 2016)= (GMRT)
Write:	<<[ACG2016] JHHMMSS.ss+DDMMSS.s>>
N:	2062
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	GMRT observations at 323 and 608 MHz of N=2062 radio sources in the Taurus molecular Cloud.
in source:	NAME Taurus Cloud
Ref:	=2016MNRAS.462.2904A
by	AINSWORTH R.E. , COUGHLAN C.P., GREEN D.A., SCAIFE A.M.M., RAY T.P.
	Mon. Not. R. Astron. Soc., 462, 2904-2917 (2016)
	A GMRT survey of regions towards the Taurus molecular cloud at 323 and 608 MHz.
o	Table 3: <[ACG2016] JHHMMSS.ss+DDMMSS.s> N=2062.
=E=	Catalogue in electronic form as J/MNRAS/462/2904
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ACG95]
[ACG95]	(Aparacio+Cepa+Gallart+, 1995)
Write:	<<[ACG95] NNNN>>
N:	1959
Object:	* (SIMBAD class: Star)
in source:	Magellanic Clouds:NGC 2366 = NGC 2366
Ref:	=1995AJ....110..212A
by	APARICIO A. , CEPA J., GALLART C., CASTANEDA H.O., CHIOSI C., BERTELLI G., MAS-HESSE J.M., MUNOZ-TUNON C., TELLES E., TENORIO-TAGLE G., DIAZ A.I., GARCIA-VARGAS M.L., GARZON F., GONZALEZ-DELGADO R.M., PEREZ E., RODRIGUEZ-ESPINOSA J.M., TERLEVICH E., TERLEVICH R.J., VARELA A.M., VILCHEZ J.M.
	Astron. J., 110, 212-222 (1995)
	Bright stars and recent star formation in the irregular Magellanic galaxy NGC 2366.
o	Table 3: <[ACG95] NNNN> N=1959
=E=	Catalogue in electronic form as J/AJ/110/212
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ACH
ACH	(Auriere+Coupinot+Hecquet)= (ACH92) = (AU)
Write:	<<ACH NN>>
N:	15
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Note:	Table 3 and 4: format 'NN'
in source:	M 31 = NGC 224
Ref:	=1992A&A...256...95A
by	AURIERE M. , COUPINOT G., HECQUET J.
	Astron. Astrophys., 256, 95-103 (1992)
	New globular clusters in the bulge of M 31.
o	Tables 2,3, col(1): The ID CMMSSDDMMm is not used in SIMBAD.
o	Tables 2,3, col(1): <C MMSSDDMMm> N=34. Tables 3, 4, col(2),(1): <ACH NN> (Nos 1-15).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [ACH2021]
[ACH2021]	(Akhter+Cunningham+Harvey-Smith+, 2021)
Write:	<<[ACH2021] Cluster-N>> <<[ACH2021] GLLL.lll+BB.bbb NN>>
N:	3+42
Object:	Cluster of dense molecular cores + Poss. Star-forming clump (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=42 candidate star-forming clumps grouped into N=3 clusters of dense molecular cores. Use of H2O Southern Galactic Plane Survey (HOPS) NH3 data.
Ref:	=2021MNRAS.502.5896A
by	AKHTER S. , CUNNINGHAM M.R., HARVEY-SMITH L., NAWAZ M.A., JONES P.A., WALSH A., DE GOUVEIA DAL PINO E.M., FALCETA-GONCALVES D.
	Mon. Not. R. Astron. Soc., 502, 5896-5920 (2021)
	Do dense molecular cores with broad emission spectra at \|l\| ≃ 5.4°, \|b\| ≃ 0.4° trace the Galactic bar? A multimolecular line study from HOPS.
o	Fig. 1: <[ACH2021] Cluster-N> (Nos 1-3). Table 2: <[ACH2021] GLLL.lll+BB.bbb NN> N=42.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ACH92
ACH92	(Auriere+Coupinot+Hecquet, 1992)
*****	Avoid the usage of ACH92, prefer ACH
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [ACH99]
[ACH99]	(Appleton+Charmandaris+Horellou+, 1999) (Not yet in Simbad)
Write:	<<[ACH99] Knot W>> <<[ACH99] Knot N>>
N:	3+8
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
Note:	ISO and NRAO VLA observations of Zw VII 466. Table 1: N=3 main regions or knots in Zw VII 466, (Nos N, E, W). Table 4: N=8 H-alpha ring knots (Nos 1-8).
in source:	ZW VII 466
Ref:	=1999ApJ...527..143A
by	APPLETON P.N. , CHARMANDARIS V., HORELLOU C., MIRABEL I.F., GHIGO F., HIGDON J.L., LORD S.
	Astrophys. J., 527, 143-153 (1999)
	Plasma and warm dust in the collisional ring galaxy VII Zw 466 from VLA and ISO observations.
o	Fig.1: G1, G2, B1 = [ACS96] G1, G2, B1. Table 3: Antennae knots A, B, Z = [VMA96] A, B, Z.
o	Table 1: <[ACH99] Knot W> (Nos N, E, W). Table 4: <[ACH99] Knot N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ACIS
ACIS	(ACIS camera aboard Chandra)
*****	Avoid the usage of ACIS, prefer [BFT2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ACIS
ACIS	(ACIS camera aboard Chandra)
*****	Avoid the usage of ACIS, prefer [FMS2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ACL2005]
[ACL2005]	(Agafonova+Centurion+Levshakov+, 2005)
Write:	<<[ACL2005] QSO J0942-1104 abs N.NNNN>>
N:	1
Object:	Absorber
Note:	The absorption system towards HE 0940-1050 = QSO J0942-1104 is new.
Ref:	=2005A&A...441....9A
by	AGAFONOVA I.I. , CENTURION M., LEVSHAKOV S.A., MOLARO P.
	Astron. Astrophys., 441, 9-None (2005)
	Spectral energy distribution of the metagalactic ionizing radiation field from QSO absorption spectra.
o	paragr.3.3: <[ACL2005] QSO J0942-1104 abs N.NNNN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ACL97]
[ACL97]	(Avruch+Cohen+Lehar+, 1997)
Write:	<<[ACL97] GW>> <<[ACL97] GWW>> <<[ACL97] Lobe W>> <<[ACL97] Arc AN>>
N:	3+2+2
Object:	? (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio maps of the QSO 0957+561: The galaxy G = YGKOW G1 = [BFT97] G1, its extension being: 'GE', 'GN', 'GNE' Detection of 2 lobes of emission, 'Lobe N' and 'Lobe S' Detection of an arc of emission: 'Arc R1', and of the brightest component of an arclike structure to the southeast of G: 'Arc R2' See also YGKOW, [RGH85], [GWC92], [BTK93], [BFT97], [BLF99], [PMN99], [SOS99], [TF99].
in source:	QSO B0957+561
Ref:	=1997ApJ...488L.121A
by	AVRUCH I.M. , COHEN A.S., LEHAR J., CONNER S.R., HAARSMA D.B., BURKE B.F.
	Astrophys. J., 488, 121-124 (1997)
	Low surface brightness radio structure in the field of gravitational lens 0957+561.
o	Galaxy G = YGKOW G1 = [BFT97] G1. Figs and text: A, B, E, BN = [RGH85] A, B, E, BN
o	<[ACL97] GWW> (Nos GE, GN, GNE), <[ACL97] Lobe W> (Nos N, S), <[ACL97] Arc RN> (Nos R1-R2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ACM2000]
[ACM2000]	(Aussel+Coia +Mazzei+, 2000)
Write:	<<[ACM2000] N-NN A>>
N:	117
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Table 2, Figs 4: N=117 ISOCAM sources observed toward 92 [HH87] point sources. Format 'N-NN A' where 'N-NN' is the format of the [HH87] source, and 'A' the different sources observed in each [HH87] field (finding charts Figs 4). Coordinates given in table 2 are those of the 'A' sources. See also the galaxies in each source: [DMB2006].
Ref:	=2000A&AS..141..257A
by	AUSSEL H. , COIA D., MAZZEI P., DE ZOTTI G., FRANCESCHINI A.
	Astron. Astrophys., Suppl. Ser., 141, 257-283 (2000)
	ISOCAM observations of the very deep IRAS 60 micron sample in the NEP region. I. The data.
o	IRAS-FSS names given in Table-I are NOT in the IRAS Faint Source Catalog of 173,044 point sources (Cat. II/156)
o	Table 2, Figs 4: <[ACM2000] N-NN A> N=117.
=E=	Catalogue in electronic form as J/A+AS/141/257
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ACM2014]
[ACM2014]	(Aberasturi+Caballero+Montesinos+, 2014)
Write:	<<[ACM2014] JHHMM+DDMM>>
N:	27
Object:	* (SIMBAD class: Star)
Note:	INT IDS observations of N=27 M dwarf candidates, in a CMC14 and 2MASS cross-match using VO tools.
Ref:	=2014AJ....148...36A
by	ABERASTURI M. , CABALLERO J.A., MONTESINOS B., GALVEZ-ORTIZ M.C., SOLANO E., MARTIN E.L.
	Astron. J., 148, 36 (2014)
	Search for bright nearby M dwarfs with virtual observatory tools.
o	Table 2: <[ACM2014] JHHMM+DDMM> N=27. Paragr. 3.6: <Koenigstuhl N> (No. 7) added.
o	Misprints: NLTT 6896 = NLTT 6496 ; G 34-53 = G 34-23 ; J2259+3738 = J2259+3736 ; in Table 5: J1574+2241 = J1547+2241.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ACM93]
[ACM93]	(Abraham+Crawford+Merrifield+, 1993)
Write:	<<[ACM93] CN>> <<[ACM93] UN>>
N:	4+3
Object:	Feature (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Different features around AO 0235+164
in source:	AO 0235+16
Ref:	=1993ApJ...415..101A
by	ABRAHAM R.G. , CRAWFORD C.S., MERRIFIELD M.R., HUTCHINGS J.B., McHARDY I.M.
	Astrophys. J., 415, 101-112 (1993)
	Is the BL Lacertae object AO 0235+164 being lensed by its intervening Mg II absorber ?
o	galaxy G = [SFK88] G2
o	Fig.3: <[ACM93] CN> (Nos C1-C4), <[ACM93] UN> (Nos U1-U3)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ACN2006]
[ACN2006]	(Aguerri+Castro-Rodriguez+Napolitano+, 2006)
Write:	<<[ACN2006] HCG 44-ESNN>>
N:	12
Object:	Em. Obj. (SIMBAD class: EmObj = Emission Object)
Stat:	is completely incorporated in Simbad
Note:	INT WFC observations of HCG 44. N=12 emission line objects are found, none associated with the group galaxies.
in source:	HCG 44
Ref:	=2006A&A...457..771A
by	AGUERRI J.A.L. , CASTRO-RODRIGUEZ N., NAPOLITANO N., ARNABOLDI M., GERHARD O.
	Astron. Astrophys., 457, 771-778 (2006)
	Diffuse light in Hickson compact groups: the dynamically young system HCG 44.
o	Table 2: <[ACN2006] HCG 44-ESNN> (Nos ES1 to ES12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ACO
ACO	(Abell+Corwin+Olowin)= A = ABCG = (Abel) = (Abell) = (ABGC) = (AC) = (S)
Write:	<<ACO NNNN>> <<ACO S NNNN>>
N:	4076+1174
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	All-sky ACO catalog: revision of Abell's northern catalog (1958ApJS....3..211A) and new southern catalogs. Table 3: (Nos 1-2712), revised northern clusters Table 4: (Nos 2713-4076), southern clusters Table 5: (Nos 1-1174), format 'S NNNN', supplementary southern clusters
Ref:	=1989ApJS...70....1A
by	ABELL G.O. , CORWIN H.G.Jr, OLOWIN R.P.
	Astrophys. J., Suppl. Ser., 70, 1-138 (1989)
	A catalog of rich clusters of galaxies.
o	Tables 3,4: <ACO NNNN> (Nos 1-4076). Table 5: <ACO S NNNN> (Nos 1-1174).
=E=	Catalogue in electronic form as VII/110
Details on Acronym: ACO
ACO	(Antlia Compact Object)
*****	Avoid the usage of ACO, prefer [CBR2013]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ACO
ACO	(Abell+Corwin+Olowin)
*****	Avoid the usage of ACO, prefer [FMV2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ACO2004]
[ACO2004]	(Anandarao+Chakraborty+Ojha+, 2004)
Write:	<<[ACO2004] SN>> <<[ACO2004] Knot-WW>>
N:	5+2
Object:	G in ClG + Knot (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Stat:	is completely incorporated in Simbad
Note:	Mt Abu, TNG and 2MASS observations. NIR images and spectra of IRAS 06061+2151: N=5 sources, stars in the cluster IRAS 06061+2151, and N=2 knots observed in H2 and Br-gamma.
in source:	IRAS 06061+2151
Ref:	=2004A&A...421.1045A
by	ANANDARAO B.G. , CHAKRABORTY A., OJHA D.K., TESTI L.
	Astron. Astrophys., 421, 1045-1050 (2004)
	Detection of knots and jets in IRAS 06061+2151.
o	6 9 5.2 +21 50 56
o	Fig.1, Table 1: <[ACO2004] AN> (Nos S1-S5). Fig.4: <[ACO2004] Knot-WW> (Nos NW, SE).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ACR98]
[ACR98]	(Ayala+Curiel+Raga+, 1998)
Write:	<<[ACR98] Jet>> <<[ACR98] A>>
N:	1+4
Object:	Part of Nebula (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Figs 1 and 2: N=1 'Jet' and N=4 Knots or Condensations (Nos A-D) in the nebula located in IRAS 20126+4104 region.
Ref:	=1998A&A...332.1055A
by	AYALA S. , CURIEL S., RAGA A.C., NORIEGA-CRESPO A., SALAS L.
	Astron. Astrophys., 332, 1055-1063 (1998)
	Near infrared imaging and spectroscopy of the IRAS 20126+4104 region.
o	Figs 1 and 2: <[ACR98] Jet>, <[ACR98] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ACRS
ACRS	(Astrographic Catalog Reference Stars)
Write:	<<ACRS NNNNNN>> <<ACRS JHHMMSS.ss+DDMMSS.s>>
N:	320211
Object:	* (SIMBAD class: Star)
Note:	NASA, NSSDC 91-10 (1991), Corbin + Urban + Warren Part 1: (Nos 1-250052) and Part 2: (500001-570159)
Auth.:	CORBIN T.E.+
=E=	Catalogue in electronic form as I/171
Details on Acronym: ACS
ACS	(Advanced Camera for Surveys)
*****	Avoid the usage of ACS, prefer [FMK2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ACS
ACS	(Advanced Camera for Surveys)
*****	Avoid the usage of ACS, prefer UDF
Origin	of the Acronym: L (2005AJ....130....1T)
Details on Acronym: ACS-GC
ACS-GC	(Advanced Camera for Surveys - General Catalog)
Write:	<<ACS-GC NNNNNNNN>>
N:	469501
Object:	* + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	The Advanced Camera for Surveys General Catalog (ACS-GC) is a photometric and morphological database using publicly available data obtained with the HST Advanced Camera for Surveys. It includes about 470000 astronomical sources (stars+galaxies) derived from the AEGIS, COSMOS, GEMS and GOODS surveys.
Ref:	=2012ApJS..200....9G
by	GRIFFITH R.L. , COOPER M.C., NEWMAN J.A., MOUSTAKAS L.A., STERN D., COMERFORD J.M., DAVIS M., LOTZ J.M., BARDEN M., CONSELICE C.J., CAPAK P.L., FABER S.M., KIRKPATRICK J.D., KOEKEMOER A.M., KOO D.C., NOESKE K.G., SCOVILLE N., SHETH K., SHOPBELL P., WILLMER C.N.A., WEINER B.
	Astrophys. J., Suppl. Ser., 200, 9 (2012)
	The Advanced Camera for Surveys General Catalog: structural parameters for approximately half a million galaxies.
o	Catalog: <ACS-GC NNNNNNNN> N=469501 among (Nos 10000007-90227432).
=E=	Catalogue in electronic form as <J/ApJS/200/9/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ACS2012]
[ACS2012]	(Alaghband-Zadeh+Chapman+Swinbank+, 2012)
Write:	<<[ACS2012] RG JHHMM+DDMMa>> <<[ACS2012] SMM JHHMM+DDMMa>>
N:	2+7+12
Object:	smm G (SIMBAD class: Galaxy)
Note:	Gemini-North NIFS and VLT SINFONI spectroscopy of submillimetre luminous galaxies. The ending "a" in format indicates individual components.
Ref:	=2012MNRAS.424.2232A
by	ALAGHBAND-ZADEH S. , CHAPMAN S.C., SWINBANK A.M., SMAIL I., HARRISON C.M., ALEXANDER D.M., CASEY C.M., DAVE R., NARAYANAN D., TAMURA Y., UMEHATA H.
	Mon. Not. R. Astron. Soc., 424, 2232-2248 (2012)
	Integral field spectroscopy of 2.0< z<2.7 submillimetre galaxies: gas morphologies and kinematics.
o	Tables 1-2: <[ACS2012] RG JHHMM+DDMM> N=2, <[ACS2012] SMM JHHMM+DDMM> N=7. Figs 3-4: <[ACS2012] SMM JHHMM+DDMMa> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ACS2013]
[ACS2013]	(Alaghband-Zadeh+Chapman+Swinbank+, 2013)
Write:	<<[ACS2013] SXDF4a>>
N:	2
Object:	smm G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Plateau de Bure Interferometer CI(1-0) and CO(4-3) observations of submillimeter galaxies. See also [ACS2012].
in source:	[CCM2006] SXDF850.4
Ref:	=2013MNRAS.435.1493A
by	ALAGHBAND-ZADEH S. , CHAPMAN S.C., SWINBANK A.M., SMAIL I., DANIELSON A.L.R., DECARLI R., IVISON R.J., MEIJERINK R., WEISS A., VAN DER WERF P.P.
	Mon. Not. R. Astron. Soc., 435, 1493-1510 (2013)
	Using [CI] to probe the interstellar medium in z ~ 2.5 sub-millimeter galaxies.
o	p.1495, 1749-096 is a probable misprint for (QSO B)1749+096. ID 141 = H-ATLAS J142413.9+022304 in Simbad. SA 22.96 = NAME SMM J221804.42+002154.4 in Simbad.
o	Fig. 3, Table 1: <[ACS2013] SXDF4a> (Nos a-b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ACS2016]
[ACS2016]	(Asboth+Conley+Sayers+, 2016)= (HELMS)
Write:	<<[ACS2016] HELMS RED NNN>> <<[ACS2016] HELMS_RED_NNN>> (not recognised by Simbad, but found in literature)
N:	477
Object:	(FIR) (SIMBAD class: FarIR = Far-IR source (λ >= 30 µm))
Note:	N=477 objects with SPIRE flux densities S₅₀₀>S₃₅₀>S-250_ and a 5σ cut-off S₅₀₀>52mJy. Use of maps from the Herschel Multi-tiered Extragalactic Survey (HerMES) Large Mode Survey (HeLMS).
Ref:	=2016MNRAS.462.1989A
by	ASBOTH V. , CONLEY A., SAYERS J., BETHERMIN M., CHAPMAN S.C., CLEMENTS D.L., COORAY A., DANNERBAUER H., FARRAH D., GLENN J., GOLWALA S.R., HALPERN M., IBAR E., IVISON R.J., MALONEY P.R., MARQUES-CHAVES R., MARTINEZ-NAVAJAS P.I., OLIVER S.J., PEREZ-FOURNON I., RIECHERS D.A., ROWAN-ROBINSON M., SCOTT D., SIEGEL S.R., VIEIRA J.D., VIERO M., WANG L., WARDLOW J., WHEELER J.
	Mon. Not. R. Astron. Soc., 462, 1989-2000 (2016)
	HerMES: a search for high-redshift dusty galaxies in the HerMES Large Mode Survey - catalogue, number counts and early results.
o	Table 2: <[ACS2016] HELMS RED NNN> (Nos 1-477).
=E=	Catalogue in electronic form as <J/MNRAS/462/1989/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ACS96]
[ACS96]	(Appleton+Charmandaris+Struck, 1996)= (G)
Write:	<<[ACS96] GN>> <<[ACS96] BN>>
N:	4+1
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Fig. 1: Map. 'B1' is a background galaxy, first observed by R. Lynds.
in source:	NAME ZW VII 466 GROUP
Ref:	=1996ApJ...468..532A
by	APPLETON P.N. , CHARMANDARIS V., STRUCK C.
	Astrophys. J., 468, 532-542 (1996)
	The head-on collision between two gas-rich galaxies: neutral hydrogen debris from the centrally smooth ring galaxy VII Zw 466.
o	Table 1: <[ACS96] GN> (Nos G1-G4). Fig.2: <[ACS96] BN> (No. B1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ACSRG
ACSRG	(Additional Catalog of Southern Ringed Galaxies)
Write:	<<ACSRG NNN>>
N:	175
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Table 6, col. (2)
Ref:	=1995ApJS...96...39B
by	BUTA R.
	Astrophys. J., Suppl. Ser., 96, 39-116 (1995)
	The catalog of southern ringed galaxies.
o	(Erratum) Erratum 1995 ApJS 98, p. 739
o	Table 3, col.(2): <CSRG NNNN> N=1235, Table 6, col.(2): <ACSRG NNN> N=175.
=E=	Catalogue in electronic form as J/ApJS/96/39
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ACSVCS
ACSVCS	(ACS camera, Virgo Cluster Survey)
Write:	<<ACSVCS NNN>>
N:	100
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	HST ACS observations of the Virgo Cluster.
in source:	NAME Virgo Cluster
Ref:	=2004ApJS..153..223C
by	COTE P. , BLAKESLEE J.P., FERRARESE L., JORDAN A., MEI S., MERRITT D., MILOSAVLJEVIC M., PENG E.W., TONRY J.L., WEST M.J.
	Astrophys. J., Suppl. Ser., 153, 223-242 (2004)
	The ACS Virgo cluster survey. I. Introduction to the survey.
o	Table 1, col(1): <ACSVCS NNN> (Nos 1-100).
=E=	Catalogue in electronic form as J/ApJS/153/223
Origin	of the Acronym: L (2008ApJ...680..154G)
Details on Acronym: ACT
ACT	(Astrographic Catalogue, Tycho)
Note:	The motivation of this catalogue was to provide accurate proper
**	catalog: use Tyc
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ACT-CL
ACT-CL	(Atacama Cosmology Telescope - Galaxy Cluster)
Write:	<<ACT-CL JHHMM+DDMM>> <<ACT-CL JHHMM.m+DDMM>>
N:	23+68+182+4195
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	Galaxy clusters detected by the Sunyaev-Zeldovich (SZ) effect by the ACT (Atacama Cosmology Telescope) at 148GHz. Follow-up observations in the optical with SOAR 4.1m telescope SOI and NTT EFOSC, and in the near-infrared with APO ARC 3.5m telescope. DR3 (2018ApJS..235...20H): N=182 DR5 (2021ApJS..253....3H) : N=4195 Data available at the NASA Legacy Archive for Microwave Background Data (LAMBDA): https://lambda.gsfc.nasa.gov/product/act/ See also ACT-S, <ACT-T>.
Ref:	=2010ApJ...723.1523M
by	MENANTEAU F. , GONZALEZ J., JUIN J.-B., MARRIAGE T.A., REESE E.D., ACQUAVIVA V., AGUIRRE P., APPEL J.W., BAKER A.J., BARRIENTOS L.F., BATTISTELLI E.S., BOND J.R., DAS S., DESHPANDE A.J., DEVLIN M.J., DICKER S., DUNKLEY J., DUNNER R., ESSINGER-HILEMAN T., FOWLER J.W., HAJIAN A., HALPERN M., HASSELFIELD M., HERNANDEZ-MONTEAGUDO C., HILTON M., HINCKS A.D., HLOZEK R., HUFFENBERGER K.M., HUGHES J.P., INFANTE L., IRWIN K.D., KLEIN J., KOSOWSKY A., LIN Y.-T., MARSDEN D., MOODLEY K., NIEMACK M.D., NOLTA M.R., PAGE L.A., PARKER L., PARTRIDGE B., SEHGAL N., SIEVERS J., SPERGEL D.N., STAGGS S.T., SWETZ D., SWITZER E., THORNTON R., TRAC H., WARNE R., WOLLACK E.
	Astrophys. J., 723, 1523-1541 (2010)
	The Atacama Cosmology Telescope: physical properties and purity of a galaxy cluster sample selected via the Sunyaev-Zel'dovich effect.
o	Tables 2-6: <ACT-CL JHHMM+DDMM> N=23. Tables 2-3: <[MGJ2010] JHHMMSS.s+DDMMSS.s> N=23.
Ref:	=2013ApJ...765...67M
by	MENANTEAU F. , SIFON C., BARRIENTOS L.F., BATTAGLIA N., BOND J.R., CRICHTON D., DAS S., DEVLIN M.J., DICKER S., DUNNER R., GRALLA M., HAJIAN A., HASSELFIELD M., HILTON M., HINCKS A.D., HUGHES J.P., INFANTE L., KOSOWSKY A., MARRIAGE T.A., MARSDEN D., MOODLEY K., NIEMACK M.D., NOLTA M.R., PAGE L.A., PARTRIDGE B., REESE E.D., SCHMITT B.L., SIEVERS J., SPERGEL D.N., STAGGS S.T., SWITZER E., WOLLACK E.J.
	Astrophys. J., 765, 67 (2013)
	The Atacama Cosmology Telescope: physical properties of Sunyaev-Zel'dovich effect clusters on the celestial equator.
o	Tables 2-5: <ACT-CL JHHMM.m+DDMM> N=68.
Ref:	=2018ApJS..235...20H
by	HILTON M. , HASSELFIELD M., SIFON C., BATTAGLIA N., AIOLA S., BHARADWAJ V., BOND J.R., CHOI S.K., CRICHTON D., DATTA R., DEVLIN M.J., DUNKLEY J., DUNNER R., GALLARDO P.A., GRALLA M., HINCKS A.D., HO S.-P.P., HUBMAYR J., HUFFENBERGER K.M., HUGHES J.P., KOOPMAN B.J., KOSOWSKY A., LOUIS T., MADHAVACHERIL M.S., MARRIAGE T.A., MAURIN L., McMAHON J., MIYATAKE H., MOODLEY K., NAESS S., NATI F., NEWBURGH L., NIEMACK M.D., OGURI M., PAGE L.A., PARTRIDGE B., SCHMITT B.L., SIEVERS J., SPERGEL D.N., STAGGS S.T., TRAC H., VAN ENGELEN A., VAVAGIAKIS E.M., WOLLACK E.J.
	Astrophys. J., Suppl. Ser., 235, 20-20 (2018)
	The Atacama Cosmology Telescope: the two-season ACTPol Sunyaev-Zel'dovich effect selected cluster catalog.
o	<ACT-CL JHHMM.m+DDMM> N=182.
Ref:	=2021ApJS..253....3H
by	HILTON M. , SIFON C., NAESS S., MADHAVACHERIL M., OGURI M., ROZO E., RYKOFF E., ABBOTT T.M.C., ADHIKARI S., AGUENA M., AIOLA S., ALLAM S., AMODEO S., AMON A., ANNIS J., ANSARINEJAD B., AROS-BUNSTER C., AUSTERMANN J.E., AVILA S., BACON D., BATTAGLIA N., BEALL J.A., BECKER D.T., BERNSTEIN G.M., BERTIN E., BHANDARKAR T., BHARGAVA S., BOND J.R., BROOKS D., BURKE D.L., CALABRESE E., CARRASCO KIND M., CARRETERO J., CHOI S.K., CHOI A., CONSELICE C., DA COSTA L.N., COSTANZI M., CRICHTON D., CROWLEY K.T., DUNNER R., DENISON E.V., DEVLIN M.J., DICKER S.R., DIEHL H.T., DIETRICH J.P., DOEL P., DUFF S.M., DUIVENVOORDEN A.J., DUNKLEY J., EVERETT S., FERRARO S., FERRERO I., FERTE A., FLAUGHER B., FRIEMAN J., GALLARDO P.A., GARCIA-BELLIDO J., GAZTANAGA E., GERDES D.W., GILES P., GOLEC J.E., GRALLA M.B., GRANDIS S., GRUEN D., GRUENDL R.A., GSCHWEND J., GUTIERREZ G., HAN D., HARTLEY W.G., HASSELFIELD M., HILL J.C., HILTON G.C., HINCKS A.D., HINTON S.R., HO S.-P.P., HONSCHEID K., HOYLE B., HUBMAYR J., HUFFENBERGER K.M., HUGHES J.P., JAELANI A.T., JAIN B., JAMES D.J., JELTEMA T., KENT S., KNOWLES K., KOOPMAN B.J., KUEHN K., LAHAV O., LIMA M., LIN Y.-T., LOKKEN M., LOUBSER S.I., MacCRANN N., MAIA M.A.G., MARRIAGE T.A., MARTIN J., McMAHON J., MELCHIOR P., MENANTEAU F., MIQUEL R., MIYATAKE H., MOODLEY K., MORGAN R., MROCZKOWSKI T., NATI F., NEWBURGH L.B., NIEMACK M.D., NISHIZAWA A.J., OGANDO R.L.C., ORLOWSKI-SCHERER J., PAGE L.A., PALMESE A., PARTRIDGE B., PAZ-CHINCHON F., PHAKATHI P., PLAZAS A.A., ROBERTSON N.C., ROMER A.K., CARNERO ROSELL A., SALATINO M., SANCHEZ E., SCHAAN E., SCHILLACI A., SEHGAL N., SERRANO S., SHIN T., SIMON S.M., SMITH M., SOARES-SANTOS M., SPERGEL D.N., STAGGS S.T., STORER E.R., SUCHYTA E., SWANSON M.E.C., TARLE G., THOMAS D., TO C., TRAC H., ULLOM J.N., VALE L.R., VAN LANEN J., VAVAGIAKIS E.M., DE VICENTE J., WILKINSON R.D., WOLLACK E.J., XU Z., ZHANG Y.
	Astrophys. J., Suppl. Ser., 253, 3-3 (2021)
	The Atacama Cosmology Telescope: a catalog of >4000 Sunyaev-Zel'dovich galaxy clusters.
o	<ACT-CL JHHMM.m+DDMM> N=4195.
=E=	Catalogue in electronic form as <J/ApJS/253/3/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ACT-S
ACT-S	(Atacama Cosmology Telescope - Extragalactic Source)
Write:	<<ACT-S JHHMMSS+DDMMSS>>
N:	157+191
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Catalog of extragalactic sources detected by the Atacama Cosmology Telescope at 148 and/or 218GHz in the 2008 Southern survey. See also ACT-CL, ACT-T>.
Ref:	=2011ApJ...731..100M
by	MARRIAGE T.A. , JUIN J.B., LIN Y.-T., MARSDEN D., NOLTA M.R., PARTRIDGE B., ADE P.A.R., AGUIRRE P., AMIRI M., APPEL J.W., BARRIENTOS L.F., BATTISTELLI E.S., BOND J.R., BROWN B., BURGER B., CHERVENAK J., DAS S., DEVLIN M.J., DICKER S.R., DORIESE W.B., DUNKLEY J., DUNNER R., ESSINGER-HILEMAN T., FISHER R.P., FOWLER J.W., HAJIAN A., HALPERN M., HASSELFIELD M., HERNANDEZ-MONTEAGUDO C., HILTON G.C., HILTON M., HINCKS A.D., HLOZEK R., HUFFENBERGER K.M., HUGHES D.H., HUGHES J.P., INFANTE L., IRWIN K.D., KAUL M., KLEIN J., KOSOWSKY A., LAU J.M., LIMON M., LUPTON R.H., MARTOCCI K., MAUSKOPF P., MENANTEAU F., MOODLEY K., MOSELEY H., NETTERFIELD C.B., NIEMACK M.D., PAGE L.A., PARKER L., QUINTANA H., REID B., SEHGAL N., SHERWIN B.D., SIEVERS J., SPERGEL D.N., STAGGS S.T., SWETZ D.S., SWITZER E.R., THORNTON R., TRAC H., TUCKER C., WARNE R., WILSON G., WOLLACK E., ZHAO Y.
	Astrophys. J., 731, 100 (2011)
	The Atacama Cosmology Telescope: extragalactic sources at 148 GHz in the 2008 survey.
o	Table A1: <ACT-S JHHMMSS+DDMMSS> N=157.
Ref:	=2014MNRAS.439.1556M
by	MARSDEN D. , GRALLA M., MARRIAGE T.A., SWITZER E.R., PARTRIDGE B., MASSARDI M., MORALES G., ADDISON G., BOND J.R., CRICHTON D., DAS S., DEVLIN M., DUNNER R., HAJIAN A., HILTON M., HINCKS A., HUGHES J.P., IRWIN K., KOSOWSKY A., MENANTEAU F., MOODLEY K., NIEMACK M., PAGE L., REESE E.D., SCHMITT B., SEHGAL N., SIEVERS J., STAGGS S., SWETZ D., THORNTON R., WOLLACK E.
	Mon. Not. R. Astron. Soc., 439, 1556-1574 (2014)
	The Atacama Cosmology Telescope: dusty star-forming galaxies and active galactic nuclei in the Southern survey.
o	Table 4: <ACT-S JHHMMSS+DDMMSS> N=191.
=E=	Catalogue in electronic form as <J/ApJ/731/100/>
=E=	Catalogue in electronic form as <J/MNRAS/439/1556/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ACT-T
ACT-T	(Atacama Cosmology Telescope - Transient)
Write:	<<ACT-T JHHMMSS+DDMMSS>>
Object:	Transient (SIMBAD class: Transient = Transient Event)
Note:	Transient millimeter-wave sources detected by the Atacama Cosmology Telescope (ACT). See also ACT-CL, ACT-S>.
Ref:	=2021ApJ...915...14N
by	NAESS S. , BATTAGLIA N., BOND J.R., CALABRESE E., CHOI S.K., COTHARD N.F., DEVLIN M., DUELL C.J., DUIVENVOORDEN A.J., DUNKLEY J., DUNNER R., GALLARDO P.A., GRALLA M., GUAN Y., HALPERN M., HILL J.C., HILTON M., HUFFENBERGER K.M., KOOPMAN B.J., KOSOWSKY A.B., MADHAVACHERIL M.S., McMAHON J., NATI F., NIEMACK M.D., PAGE L., PARTRIDGE B., SALATINO M., SEHGAL N., SPERGEL D., STAGGS S., WOLLACK E.J., XU Z.
	Astrophys. J., 915, 14-14 (2021)
	The Atacama Cosmology Telescope: detection of millimeter-wave transient sources.
o	Table 1: <ACT-T JHHMMSS+DDMMSS> N=3.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ACZ2018]
[ACZ2018]	(Acebron+Cibirka+Zitrin+, 2018)
Write:	<<[ACZ2018] MACS J0308 N.N>> <<[ACZ2018] MACS J0308 cN.N>> <<[ACZ2018] MACS J0308 c4.3b>> <<[ACZ2018] PLCK G171.9 N.N>> <<[ACZ2018] PLCK G171.9 cN.N>>
N:	7+5+1+9+11
Object:	Grav. lensed image of a G + Grav. lensed image + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=7+9 gravitationally lensed images and N=5+1 gravitationally lensed image candidates by the galaxy clusters MCS J0308.9+2645 and PLCKESZ G171.94-40.65 respectively. N=1 additional galaxy in the field of MCS J0308.9+2645. Use of data from the RELICS Hubble Treasury program. See also [AAZ2019], [CAZ2018], [CSA2018], [PSC2018].
in source:	MCS J0308.9+2645
in source:	PLCKESZ G171.94-40.65
Ref:	=2018ApJ...858...42A
by	ACEBRON A. , CIBIRKA N., ZITRIN A., COE D., AGULLI I., SHARON K., BRADAC M., FRYE B., LIVERMORE R.C., MAHLER G., SALMON B., UMETSU K., BRADLEY L., ANDRADE-SANTOS F., AVILA R., CARRASCO D., CERNY C., CZAKON N.G., DAWSON W.A., HOAG A.T., HUANG K.-H., JOHNSON T.L., JONES C., KIKUCHIHARA S., LAM D., LOVISARI L., MAINALI R., OESCH P.A., OGAZ S., OUCHI M., PAST M., PATERNO-MAHLER R., PETERSON A., RYAN R.E., SENDRA-SERVER I., STARK D.P., STRAIT V., TOFT S., TRENTI M., VULCANI B.
	Astrophys. J., 858, 42-42 (2018)
	RELICS: strong-lensing analysis of the massive clusters MACS J0308.9+2645 and PLCK G171.9-40.7.
o	Fig. 1, Table 2: <[ACZ2018] MACS J0308 N.N> N=7 among (Nos 1.1-1.3 to 3.1-3.2), <[ACZ2018] MACS J0308 cN.N> N=5 among (Nos c4.1-c4.3 to c5.1-c5.2), <[ACZ2018] MACS J0308 c4.3b> N=1. Fig. 2, Table 3: <[ACZ2018] PLCK G171.9 N.N> N=9 among (Nos 1.1-1.3 to 3.1-3.3), <[ACZ2018] PLCK G171.9 cN.N> N=11 among (Nos c4.1-c4.3 to c7.1-c7.3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AD
AD	(Anno Domini)
*****	Avoid the usage of AD, prefer SN
Details on Acronym: [AD85]
[AD85]	(Arp+Duhalde, 1985)= (NGC 520.)
Write:	<<[AD85] NNN>> <<[AD85] DNN>>
N:	11+9
Object:	QSO (SIMBAD class: QSO = Quasar)
Note:	QSO near NGC 520 Table I: N=11 among (Nos 30-192) and N=8 among (Nos D1-D10) + No. D68, D in the format stands for Duhalde Finding chart
Ref:	=1985PASP...97.1149A
by	ARP H. , DUHALDE O.
	Publ. Astron. Soc. Pac., 97, 1149-1157 (1985)
	Quasars near NGC 520.
o	Table I: <[AD85] NNN> N=11 among (Nos 30-192), <[AD85] DNN> N=8 among (Nos D1-D10) + No. D68
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AD95]
[AD95]	(Ali+DePoy, 1995)
Write:	<<[AD95] NNNN>>
N:	3548
Object:	* (SIMBAD class: Star)
Note:	N=3548 sources in Ori A MCld Table 2: N=100 brightest nonsaturated stars
in source:	NAME Ori A
Ref:	=1995AJ....109..709A
by	ALI B. , DEPOY D.L.
	Astron. J., 109, 709-720 (1995)
	A 2.2 µ.m imaging survey of the Orion A molecular cloud.
o	About half of the sources (those having accurate positions) are included in SIMBAD.
o	Table 2: <[AD95] NNNN> N=100 among 3548
=E=	Catalogue in electronic form as J/AJ/109/709
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ADA
ADA	(A.D. Andrews)
*****	Avoid the usage of ADA, prefer Andrews
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [ADB2010]
[ADB2010]	(Adami+Durret+Benoist+, 2010)
Write:	<<[ADB2010] DN-NN>> <<[ADB2010] WN-NNN>>
N:	1200
Object:	ClG candidate (SIMBAD class: ClG_Candidate = Cluster of Galaxies Candidate)
Note:	N=1200 candidate clusters in the CFHTLS Deep and Wide fields.
Ref:	=2010A&A...509A..81A
by	ADAMI C. , DURRET F., BENOIST C., COUPON J., MAZURE A., MENEUX B., ILBERT O., BLAIZOT J., ARNOUTS S., CAPPI A., GARILLI B., GUENNOU L., LEBRUN V., LEFEVRE O., MAUROGORDATO S., McCRACKEN H.J., MELLIER Y., SLEZAK E., TRESSE L., ULMER M.P.
	Astron. Astrophys., 509A, 81-81 (2010)
	Galaxy structure searches by photometric redshifts in the CFHTLS.
o	Tables A.1-A.3: <[ADB2010] DN-NN> N=60+64+47. Tables A.4-A.6: <[ADB2010] WN-NNN> N=755+175+99.
=E=	Catalogue in electronic form as J/A+A/509/A81
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ADBS
ADBS	(Arecibo Dual-Beam Survey)
Write:	<<ADBS JHHMMSS+DDMM>>
N:	265
Object:	G (SIMBAD class: Galaxy)
Note:	The ADBS is a blind 21cm search for galaxies. N=265 among which 81 not previously cataloged optically and 11 without clear associated optical counterpart.
Ref:	=2000ApJS..130..177R
by	ROSENBERG J.L. , SCHNEIDER S.E.
	Astrophys. J., Suppl. Ser., 130, 177-199 (2000)
	The Arecibo dual-beam survey: Arecibo and VLA observations.
o	ADBS objects in table 2 are numbered 'NNN' in 2005AJ....129.1311R, and cross-id. with the designation <[RS2000] NNN> (Nos 1-265).
o	Table 2: <ADBS JHHMMSS+DDMM> N=265.
=E=	Catalogue in electronic form as J/ApJS/130/177
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ADC2016]
[ADC2016]	(Andreoni+D'avanzo+Campana+, 2016)
Write:	<<[ADC2016] {NGC}NNNN-{I\|O}N>>
N:	6
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Swift XRT and UVOT observations of N=5 transient sources in the field of five galaxies.
in source:	NGC 1084
in source:	NGC 2770
in source:	NGC 4303
in source:	NGC 3147
in source:	NGC 3690
Ref:	=2016A&A...587A.147A
by	ANDREONI I. , D'AVANZO P., CAMPANA S., BRANCHESI M., BERNARDINI M.G., DELLA VALLE M., MANNUCCI F., MELANDRI A., TAGLIAFERRI G.
	Astron. Astrophys., 587A, 147-147 (2016)
	A time domain experiment with Swift: monitoring of seven nearby galaxies.
o	Text: <[ADC2016] NGCNNNN-AN> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADC93]
[ADC93]	(Armandroff+Da Costa+Caldwell+, 1993)
Write:	<<[ADC93] NNN>>
N:	635
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	And III
Ref:	=1993AJ....106..986A
by	ARMANDROFF T.E. , DA COSTA G.S., CALDWELL N., SEITZER P.
	Astron. J., 106, 986-998 (1993)
	The dwarf spheroidal companions to M31: a color-magnitude diagram for And III.
o	<[ADC93] NNN> N=635
=E=	Catalogue in electronic form as J/AJ/106/986
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADC99]
[ADC99]	(Arnouts+D'odorico+Cristiani+, 1999)
Write:	<<[ADC99] NNN>>
N:	608
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	BVrI photometry of galaxies in a 5.62arcmin2 field 80arcsec south of the high redshift (z=4.7) quasar BR 1202-0725, derived from observations with the direct CCD camera SUSI at the ESO NTT.
Ref:	=1999A&A...341..641A
by	ARNOUTS S. , D'ODORICO S., CRISTIANI S., ZAGGIA S., FONTANA A., GIALLONGO E.
	Astron. Astrophys., 341, 641-652 (1999)
	The NTT SUSI deep field.
o	Catalogue: <[ADC99] NNN> (Nos 1-608).
=E=	Catalogue in electronic form as J/A+A/341/641
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADD2012]
[ADD2012]	(Alves+Davies+Dickinson+, 2012)
Write:	<<[ADD2012] HII NN>> <<[ADD2012] SNR NN>>
N:	48+26
Object:	HII + SNR (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=48 HII regions and N=26 SNRs in the Galactic Plane. Use of radio recombination line data from the HIPASS survey.
Ref:	=2012MNRAS.422.2429A
by	ALVES M.I.R. , DAVIES R.D., DICKINSON C., CALABRETTA M., DAVIS R., STAVELEY-SMITH L.
	Mon. Not. R. Astron. Soc., 422, 2429-2443 (2012)
	A derivation of the free-free emission on the Galactic plane between l= 20° and 44°.
o	Table 2: <[ADD2012] HII NN> (Nos 1-48). Table 4: <[ADD2012] SNR NN> (Nos 1-26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ADFS
ADFS	(AKARI Deep Field South) (Not yet in Simbad)
*****	Avoid the usage of ADFS, prefer [MPT2010]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ADG2013]
[ADG2013]	(Adami+Durret+Guennou+, 2013) (Not yet in Simbad)
Write:	<<[ADG2013] Obj 1>> <<[ADG2013] SN>>
N:	1+3
Note:	N=1 low signal-to-noise object and N=3 diffuse light sources in the cluster of galaxies ClG J1449+0856. Use of HST NICMOS H band data.
in source:	ClG J1449+0856
Ref:	=2013A&A...551A..20A
by	ADAMI C. , DURRET F., GUENNOU L., DA ROCHA C.
	Astron. Astrophys., 551A, 20-20 (2013)
	Diffuse light in the young cluster of galaxies CL J1449+0856 at z = 2.07.
o	Fig. 1: <[ADG2013] Obj 1> N=1, <[ADG2013] SN> (Nos S1-S3).
o	Obj.1 and S1-S3 are not in Simbad (no coordinates).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADG2018]
[ADG2018]	(Anderson+Dessart+Gutierrez+, 2018)
Write:	<<[ADG2018] NN>>
N:	24
Object:	* (SIMBAD class: Star)
Note:	Catalina Real-Time Transient Survey (CRTS) observations of SN 2001bc. Use of Pan-STARRS DR1 data.
in source:	SN 2015bc
Ref:	=2018NatAs...2..574A
by	ANDERSON J.P. , DESSART L., GUTIERREZ C.P., KRUHLER T., GALBANY L., JERKSTRAND A., SMARTT S.J., CONTRERAS C., MORRELL N., PHILLIPS M.M., STRITZINGER M.D., HSIAO E.Y., GONZALEZ-GAITAN S., AGLIOZZO C., CASTELLON S., CHAMBERS K.C., CHEN T.-W., FLEWELLING H., GONZALEZ C., HOSSEINZADEH G., HUBER M., FRASER M., INSERRA C., KANKARE E., MATTILA S., MAGNIER E., MAGUIRE K., LOWE T.B., SOLLERMAN J., SULLIVAN M., YOUNG D.R., VALENTI S.
	NatAs, 2, 574-579 (2018)
	The lowest-metallicity type II supernova from the highest-mass red supergiant progenitor.
o	Table 1: <[ADG2018] NN> (Nos 1-24).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADG70]
[ADG70]	(Altenhoff+Downes+Goad+, 1970) (Not yet in Simbad)
Write:	<<[ADG70] GLLL.l+B.b>>
N:	356
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	See also [ADP79].
Ref:	=1970A&AS....1..319A
by	ALTENHOFF W.J. , DOWNES D., GOAD L., MAXWELL A., RINEHART R.
	Astron. Astrophys., Suppl. Ser., 1, 319-355 (1970)
	Surveys of the galactic plane at 1.414, 2.695 and 5.000 GHz.
o	Table 2: <[ADG70] GLLL.l+B.b> N=356.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADH2006]
[ADH2006]	(Ashby+Dye+Huano+, 2006)
Write:	<<[ADH2006] 14.NN>> <<[ADH2006] 14.NNA>>
N:	31
Object:	(Mid IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Spitzer mid-IR identification candidates of SCUBA CUDSS galaxies in the 14h CUDSS field.
Ref:	=2006ApJ...644..778A
by	ASHBY M.L.N. , DYE S., HUANG J.-S., EALES S., WILLNER S.P., WEBB T.M.A., BARMBY P., RIGOPOULOU D., EGAMI E., McCRACKEN H., LILLY S., MIYAZAKI S., BRODWIN M., BLAYLOCK M., CADIEN J., FAZIO G.G.
	Astrophys. J., 644, 778-791 (2006)
	Mid-infrared identifications of SCUBA galaxies in the CUDSS 14 hour field with the Spitzer Space Telescope.
o	Table 1: <[ADH2006] 14.NN> N=8, <[ADH2006] 14.NNA> N=23.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADH2018]
[ADH2018]	(Anthony-Twarog+Deliyannis+Harmer+, 2018)
Write:	<<[ADH2018] FNN>>
N:	11
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	WIYN HYDRA 3.5m telescope spectroscopic observations of N=11 stars in M35.
in source:	NGC 2168 = M 35
Ref:	=2018AJ....156...37A
by	ANTHONY-TWAROG B.J. , DELIYANNIS C.P., HARMER D., LEE-BROWN D.B., STEINHAUER A., SUN Q., TWAROG B.A.
	Astron. J., 156, 37-37 (2018)
	Li in open clusters: cool dwarfs in the young, subsolar-metallicity cluster M35 (NGC 2168).
o	Tables 1-3: <[ADH2018] FNN> (Nos F1-F11).
=E=	Catalogue in electronic form as J/AJ/156/37
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADK2000]
[ADK2000]	(Albert+Demers+Kunkel, 2000)
Write:	<<[ADK2000] NNN>>
N:	195
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Note:	See also [BD2000], [DB2002], [LDB2002], [BDL2003], [DBL2003], [DBL2003b], [BD2004a], [BD2004b], [DBL2004].
in source:	IC 1613
Ref:	=2000AJ....119.2780A
by	ALBERT L. , DEMERS S., KUNKEL W.E.
	Astron. J., 119, 2780-2788 (2000)
	A carbon star survey of the Local Group dwarf galaxies. I. IC 1613.
o	Table 2: <[ADK2000] NNN> (Nos 1-195).
=E=	Catalogue in electronic form as J/AJ/119/2780
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADK96]
[ADK96]	(Asai+Dotani+Kunieda+, 1996)
Write:	<<[ADK96] JHHMMSS+DDMM>>
N:	1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ASCA SIS and GIS observations. N=1 weak source detected in the field of the 'Rapid Burster'.
Ref:	=1996PASJ...48L..27A
by	ASAI K. , DOTANI T., KUNIEDA H., KAWAI N.
	Publ. Astron. Soc. Jap., 48, 27-31 (1996)
	ASCA observation of the Rapid Burster in quiescence.
o	<[ADK96] JHHMMSS+DDMM> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADM2008]
[ADM2008]	(Albacete-Colombo Damiani+Micela+, 2008)
Write:	<<[ADM2008] NNNN>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS-I observations at the center of Cl Trumpler 16. See also CXOTr16.
in source:	Cl Trumpler 16
Ref:	=2008A&A...490.1055A
by	ALBACETE-COLOMBO J.F. , DAMIANI F., MICELA G., SCIORTINO S., HARNDEN F.R.Jr
	Astron. Astrophys., 490, 1055-1070 (2008)
	An X-ray survey of low-mass stars in Trumpler 16 with Chandra.
o	Table 1, col(2): the ID CXOCYG (ID for sources in the Association Cyg OB 2) is a misprint, we have created CXOTr16 for sources in Cl Trumpler 16.
o	Table 1, col(1): <[ADM2008] NNNN> (Nos 1-1035) = Table 1, col(2): <CXOTr16 JHHMMSS.ss+DDMMSS.s> N=1035.
=E=	Catalogue in electronic form as J/A+A/490/1055
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADM95]
[ADM95]	(Abraham+Dobashi+Mizuno+, 1995)= (IRAS)
Write:	<<[ADM95] A>> <<[ADM95] NN>> <<[ADM95] IRAS-N>>
N:	6+15+6
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Table 2: format 'A', (Nos A-F), N=6 clump in LDN 1188 Table 3: format 'NN', (Nos 1-15), N=15 H-alf em. obj. in LDN 1188 Table 3: format 'IRAS-N' (Nos 1-6), N=6 IR obj. in LDN 1188
in source:	LDN 1188
Ref:	=1995A&A...300..525A
by	ABRAHAM P. , DOBASHI K., MIZUNO A., FUKUI Y.
	Astron. Astrophys., 300, 525-533 (1995)
	Molecular material and young stellar objects in the L 1188 dark cloud complex.
o	Table 2: <[ADM95] A> (Nos A-F), Table 3: <[ADM95] NN> (Nos 1-15), Table 4: <[ADM95] IRAS-N> (Nos 1-6)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADM96]
[ADM96]	(Andreon+Davoust+Michard+, 1996)
Write:	<<[ADM96] anon N>> <<[ADM96] supp NN>>
N:	3+16
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Table 4: N=3 anonymous galaxies with m_R < 16.05 are added, format 'anon N' and N=16 anonymous galaxies with m_R > 16.05, format 'supp NN' Maps fig. 3.
in source:	Coma Cluster = ACO 1656
Ref:	=1996A&AS..116..429A
by	ANDREON S. , DAVOUST E., MICHARD R., NIETO J.-L., POULAIN P.
	Astron. Astrophys., Suppl. Ser., 116, 429-445 (1996)
	Morphological classification and structural parameters for early-type galaxies in the Coma cluster.
o	objects only in table 1 are not in Simbad
o	Table 4: <[ADM96] anon N> (Nos 1-3), <[ADM96] supp NN> (Nos 1-16)
=E=	Catalogue in electronic form as J/A+AS/116/429
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADM99]
[ADM99]	(Arendt+Dwek+Moseley, 1999) (Not yet in Simbad)
Write:	<<[ADM99] WN>>
N:	11
Object:	Region (SIMBAD class: Region = Region defined in the Sky)
in source:	NAME Cas A
Ref:	=1999ApJ...521..234A
by	ARENDT R.G. , DWEK E., MOSELEY S.H.
	Astrophys. J., 521, 234-245 (1999)
	Newly synthesized elements and pristine dust in the Cassiopeia A supernova remnant.
o	p. 235, knot D = [F90] D.
o	Table 1: <[ADM99] WN> (Nos N1-N6, S1-S5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADP2008]
[ADP2008]	(Andreon+De Propis+Puddu+, 2008)
Write:	<<[ADP2008] JHHMMSS.ss+DDMMSS.s>>
N:	21
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	CTIO 4m Blanco telescope observations of the galaxy cluster RzCS 52.
in source:	RzCS 052
Ref:	=2008MNRAS.383..102A
by	ANDREON S. , DE PROPRIS R., PUDDU E., GIORDANO L., QUINTANA H.
	Mon. Not. R. Astron. Soc., 383, 102-112 (2008)
	Scaling relations of the colour-detected cluster RzCS 052 at z = 1.016 and some other high-redshift clusters.
o	RzCS 058 not identified.
o	Table 1: <[ADP2008] JHHMMSS.ss+DDMMSS.s> N=21. Text: <RzCS NNN> (No. 052).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADP2010]
[ADP2010]	(Austermann+Dunlop+Perera+, 2010)= (AzLOCK) = (AzSXDF)
Write:	<<[ADP2010] AzLOCK.NN>> <<[ADP2010] AzSXDF.NN>>
N:	86+28
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	JCMT AzTEC 1.1mm continuum observations of N=86+28 sources in the Lockman Hole and SXDF fields. See also AzTEC.
in source:	NAME Lockman Hole
in source:	NAME SXDF
Ref:	=2010MNRAS.401..160A
by	AUSTERMANN J.E. , DUNLOP J.S., PERERA T.A., SCOTT K.S., WILSON G.W., ARETXAGA I., HUGHES D.H., ALMAINI O., CHAPIN E.L., CHAPMAN S.C., CIRASUOLO M., CLEMENTS D.L., COPPIN K.E.K., DUNNE L., DYE S., EALES S.A., EGAMI E., FARRAH D., FERRUSCA D., FLYNN S., HAIG D., HALPERN M., IBAR E., IVISON R.J., VAN KAMPEN E., KANG Y., KIM S., LACEY C., LOWENTHAL J.D., MAUSKOPF P.D., McLURE R.J., MORTIER A.M.J., NEGRELLO M., OLIVER S., PEACOCK J.A., POPE A., RAWLINGS S., RIEKE G., ROSEBOOM I., ROWAN-ROBINSON M., SCOTT D., SERJEANT S., SMAIL I., SWINBANK A.M., STEVENS J.A., VELAZQUEZ M., WAGG J., YUN M.S.
	Mon. Not. R. Astron. Soc., 401, 160-176 (2010)
	AzTEC half square ° survey of the SHADES fields - I. Maps, catalogues and source counts.
o	Tables 1-2, col(1): <AzTEC JHHMMSS.ss+DDMMSS.s> N=86 = Tables 1-2, col(2): <[ADP2010] AzLOCK.NN> (Nos 1-86). Table 3, col(1): <AzTEC JHHMMSS.ss+DDMMSS.s> N=28 = Table 3, col(2): <[ADP2010] AzSXDF.NN> (Nos 1-28).
=E=	Catalogue in electronic form as <J/MNRAS/401/160/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADP79]
[ADP79]	(Altenhoff+Downes+Pauls+, 1979)
Write:	<<[ADP79] LLL.lll+B.bbb>>
N:	1186
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	See also [ADG70].
Ref:	=1979A&AS...35...23A
by	ALTENHOFF W.J. , DOWNES D., PAULS T., SCHRAML J.
	Astron. Astrophys., Suppl. Ser., 35, 23-54 (1979)
	Survey of the galactic plane at 4.875 GHz.
o	Year of publication given as 1978 in the paper.
o	<[ADP79] LLL.lll+B.bbb> N=1186
=E=	Catalogue in electronic form as J/A+AS/35/23
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADR2016]
[ADR2016]	(Andreon+Dong+Raichoor, 2016)
Write:	<<[ADR2016] Abell NNNN NNNN>> <<[ADR2016] IDCS J1426.5+3508 NNNN>> <<[ADR2016] ISCS J1432.3+3253 NNNN>> <<[ADR2016] JKCS041 NNNN>> <<[ADR2016] MACSJHHMM.m+DDMM NNNN>> <<[ADR2016] RXJ0152.7-1357 NNNN>> <<[ADR2016] SpARCS J022426-032330 NNNN>> <<[ADR2016] SpARCS104922.6+564032.5 NNNN>> <<[ADR2016] SPT-CL JHHMM+DDMM NNNN>> <<[ADR2016] XDCP J0044.0-2033 NNNN>>
N:	158
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Use of HST ACS and WFC3 archival data to study N=158 galaxies in N=13 galaxy clusters.
Ref:	=2016A&A...593A...2A
by	ANDREON S. , DONG H., RAICHOOR A.
	Astron. Astrophys., 593A, 2-2 (2016)
	Size growth of red-sequence early-type galaxies in clusters in the last 10 Gyr.
o	(Erratum) erratum vol. 602, art. C1 (2017)
o	Table 3: <[ADR2016] Abell NNNN NNNN> N=44, <[ADR2016] IDCS J1426.5+3508 NNNN> N=5, <[ADR2016] ISCS J1432.3+3253 NNNN> N=3, <[ADR2016] MACSJHHMM.m+DDMM NNNN> N=44, <[ADR2016] RXJ0152.7-1357 NNNN> N=21, <[ADR2016] SpARCS104922.6+564032.5 NNNN> N=3, <[ADR2016] SpARCS J022426-032330 NNNN> N=3, <[ADR2016] SPT-CL JHHMM+DDMM NNNN> N=23, <[ADR2016] XDCP J0044.0-2033 NNNN> N=5.
=E=	Catalogue in electronic form as J/A+A/593/A2
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ADS
ADS	(Aitken, Double *)= (A) = (Aitken)
Write:	<<ADS NNNNN AAA>> <<ADS NNNNNa AAA>>
N:	17180
Object:	(SIMBAD class: = Double or Multiple Star)
Note:	See also IDS and BDS.
Ref:	=1932ADS...C......0A
by	AITKEN R.G.
	Carnegie Inst. Washington D.C. Publ. 417, 0-None (1932)
	New general catalogue of double stars within 120 ° of the North Pole.
o	<ADS NNNNNAA> N=17180.
Details on Acronym: [ADS81]
[ADS81]	(Appleton+Davies+Stephenson+, 1981)
Write:	<<[ADS81] SW Cloud>> <<[ADS81] R>>
N:	1+8
Object:	Region (SIMBAD class: Region = Region defined in the Sky)
Note:	N=1 cloud named 'SW Cloud'. N=8 emission ridges of neutral Hydrogen emission in M 81 group ('Feature R' in the paper).
in source:	NAME M 81 GROUP
Ref:	=1981MNRAS.195..327A
by	APPLETON P.N. , DAVIES R.D., STEPHENSON R.J.
	Mon. Not. R. Astron. Soc., 195, 327-352 (1981)
	The neutral hydrogen content of the M 81/M 82 group of galaxies -I. The observations.
o	Table 1, Fig.2: <[ADS81] SW Cloud> N=1. Table 3, Fig.3: <[ADS81] R> (Nos I to VIII).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADT2014]
[ADT2014]	(Anthony-Twarog+Deliyannis+Twarog, 2014)
Write:	<<[ADT2014] DDD.ddddd+DD.ddddd>>
N:	7187
Object:	* (SIMBAD class: Star)
Note:	WYIN 0.9m telescope ubvyCaHβ observations of N=7187 stars in the field of NGC 6819.
in source:	NGC 6819
Ref:	=2014AJ....148...51A
by	ANTHONY-TWAROG B.J. , DELIYANNIS C.P., TWAROG B.A.
	Astron. J., 148, 51 (2014)
	A uvbyCaHβ analysis of the old open cluster, NGC 6819.
o	Table 2: <[ADT2014] DDD.ddddd+DD.ddddd> N=7187.
=E=	Catalogue in electronic form as <J/AJ/148/51/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADT2016]
[ADT2016]	(Anthony-Twarog+Deliyannis+Twarog+, 2016) (Not yet in Simbad)
Write:	<<[ADT2016] NNNN>> <<[ADT2016] JDDD.dddddd+DD.dddddd>>
N:	921+1308
Object:	* (SIMBAD class: Star)
Note:	CTIO SMARTS observations of N=921+1308 stars in NGC 2506, as part of the WIYN open cluster study (WOCS). See also [ALD2018].
in source:	NGC 2506
Ref:	=2016AJ....152..192A
by	ANTHONY-TWAROG B.J. , DELIYANNIS C.P., TWAROG B.A.
	Astron. J., 152, 192-192 (2016)
	WIYN open cluster study. LXXII. A uvbyCaHβ CCD analysis of the metal-deficient open cluster NGC 2506.
o	Table 2: <[ADT2016] NNNN> N=921 among (Nos 1101-5387), <[ADT2016] JDDD.dddddd+DD.dddddd> N=1308.
=E=	Catalogue in electronic form as <J/AJ/152/192/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADW2016]
[ADW2016]	(Aravena+Decarli+Walter+, 2016)= ([ADW2016a]) = (ASPECS)
Write:	<<[ADW2016] CNN>> <<[ADW2016] MM JHHMMSS.ss+DDMMSS.s>>
N:	16*2
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA 1.2mm continuum observations of N=16 sources, as part of the ALMA SPECtroscopic Survey in the Hubble Ultra-Deep Field (ASPECS). See also [WDA2016] and [DWA2016].
in source:	NAME Hubble Ultra Deep Field
Ref:	=2016ApJ...833...68A
by	ARAVENA M. , DECARLI R., WALTER F., DA CUNHA E., BAUER F.E., CARILLI C.L., DADDI E., ELBAZ D., IVISON R.J., RIECHERS D.A., SMAIL I., SWINBANK A.M., WEISS A., ANGUITA T., ASSEF R.J., BELL E., BERTOLDI F., BACON R., BOUWENS R., CORTES P., COX P., GONZALEZ-LOPEZ J., HODGE J., IBAR E., INAMI H., INFANTE L., KARIM A., LE FEVRE O., MAGNELLI B., OTA K., POPPING G., SHETH K., VAN DER WERF P., WAGG J.
	Astrophys. J., 833, 68-68 (2016)
	The ALMA spectroscopic survey in the Hubble Ultra Deep Field: continuum number counts, resolved 1.2 mm extragalactic background, and properties of the faintest dusty star-forming galaxies.
o	Table 1: <[ADW2016] CNN> = <[ADW2016] MM JHHMMSS.ss+DDMMSS.s> N=16.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADW2016a]
[ADW2016a]	(Aravena+Decarli+Walter+, 2016)
*****	Avoid the usage of [ADW2016a], prefer [ADW2016]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADW2016b]
[ADW2016b]	(Aravena+Decarli+Walter+, 2016)
Write:	<<[ADW2016b] IDNN>> <<[ADW2016b] IDXNN>>
N:	50
Object:	G (SIMBAD class: Galaxy)
Note:	ALMA 1mm and 3mm continuum observations of N=56+2 optical dropout galaxies at 5.5<z<8.5 in the Hubble Ultra-deep Field (UDF). Use of the ALMA SPECtroscopic Survey in the Hubble Ultra-Deep Field (ASPECS). Use of archival HST CANDELS data. See also [BIO2015], [SRE2013], and [MDB2013].
Ref:	=2016ApJ...833...71A
by	ARAVENA M. , DECARLI R., WALTER F., BOUWENS R., OESCH P.A., CARILLI C.L., BAUER F.E., DA CUNHA E., DADDI E., GONZALEZ-LOPEZ J., IVISON R.J., RIECHERS D.A., SMAIL I., SWINBANK A.M., WEISS A., ANGUITA T., BACON R., BELL E., BERTOLDI F., CORTES P., COX P., HODGE J., IBAR E., INAMI H., INFANTE L., KARIM A., MAGNELLI B., OTA K., POPPING G., VAN DER WERF P., WAGG J., FUDAMOTO Y.
	Astrophys. J., 833, 71-71 (2016)
	The ALMA spectroscopic survey in the Hubble Ultra Deep Field: search for [CII] line and dust emission in 6 < z < 8 galaxies.
o	Table 1: <[ADW2016b] IDNN> N=58 among (Nos 2-59). Table 2: <[ADW2016b] IDXNN> N=2 (Nos IDX25, IDX34).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ADW79]
[ADW79]	(Arp+De ruiter+Willis, 1979)= (UB)
Write:	<<[ADW79] NGC 772 UB N>>
N:	1
Object:	(Blue + UV) (SIMBAD class: blue = Blue Object)
Ref:	=1979A&A....77...86A
by	ARP H.C. , DE RUITER H.R., WILLIS A.G.
	Astron. Astrophys., 77, 86-92 (1979)
	A Westerbork 1415 MHz survey of radio sources.
o	Table 1c: <[ADW79] NGC 772 UB 2> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AE
AE	(A. Elvius)
Write:	<<NAME AE N>>
N:	1
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	N=1 He-rich obj. = V* V803 Cen
Ref:	=1975A&A....44..117E
by	ELVIUS A.
	Astron. Astrophys., 44, 117-121 (1975)
	Variable blue object with a peculiar spectrum.
o	<NAME AE 1> = V* V803 Cen
Details on Acronym: Ae
Ae	(Allen)
*****	Avoid the usage of Ae, prefer Al
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [AEC2006]
[AEC2006]	(Augusto+Edge+Chandler, 2006) (Not yet in Simbad)
Write:	<<[AEC2006] B2151+174 A>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Radio imaging of the radio-galaxy [LO95] B2151+174.
Ref:	=2006MNRAS.367..366A
by	AUGUSTO P. , EDGE A.C., CHANDLER C.J.
	Mon. Not. R. Astron. Soc., 367, 366-374 (2006)
	The radio properties of the cD galaxy of Abell 2390.
o	Fig.1: <[AEC2006] B2151+174 A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AEC93]
[AEC93]	(Aragon-Salamanca+Ellis+Couch+, 1993)
Write:	<<[AEC93] HHMM+DD NNN>> <<[AEC93] HHMM+DDMM NN>> <<[AEC93] ANNNN.NNAA AN>> <<[AEC93] ANNNN.NNAA NNa>>
N:	193
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Maps in Figs 3. Objects '[AEC93] J1888.16CL NN' and '[AEC93] J1888.16CL AN' are identical to '[CSP85] NN' and '[CSP85] AN', see [CSP85]. Objects '[AEC93] 0016+16 NNN' are identical to '[ECM85] NNN', see [ECM85]
in source:	ClG 0016+1609 = 1E 0015.9+1609
in source:	CEMM J1888.16CL
in source:	ClG 0317+1521
in source:	CEMM F1767.10TC
in source:	ClG 0020+0407
in source:	ClG 1322+3027
in source:	ClG 2155+0334
in source:	ClG 1603+4313
in source:	ClG 1603+4329
Ref:	=1993MNRAS.262..764A
by	ARAGON-SALAMANCA A. , ELLIS R.S., COUCH W.J., CARTER D.
	Mon. Not. R. Astron. Soc., 262, 764-794 (1993)
	Evidence for systematic evolution in the properties of galaxies in distant clusters.
o	Objects '[AEC93] J1888.16CL NN' = '[CSP85] NN', '[AEC93] J1888.16CL AN' = '[CSP85] AN', '[AEC93] 0016+16 NNN' = '[ECM85] NNN'.
o	Table 4: <[AEC93] HHMM+DD NNN>, <[AEC93] HHMM+DDMM NN>, <[AEC93] ANNNN.NNAA NNa> N=189. Table 4: <[AEC93] J1888.16CL AN> = <[CSP85] AN> (Nos A1-A4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AEF
AEF	(Allen+Edge+Fabian+)
*****	Avoid the usage of AEF, prefer [AEF92]
Origin	of the Acronym: L (1995MNRAS.277....1S)
Details on Acronym: [AEF92]
[AEF92]	(Allen+Edge+Fabian+, 1992)= (AEF)
Write:	<<[AEF92] ACO NNNN N>>
N:	2+2+3
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	See also [CEF95], [CAE99].
in source:	ACO 1682
in source:	ACO 1703
in source:	ACO 2219
Ref:	=1992MNRAS.259...67A
by	ALLEN S.W. , EDGE A.C., FABIAN A.C., BOHRINGER H., CRAWFORD C.S., EBELING H., JOHNSTONE R.M., NAYLOR T., SCHWARZ R.A.
	Mon. Not. R. Astron. Soc., 259, 67-81 (1992)
	Optical spectroscopy of the ROSAT X-ray brightest clusters.
o	Table 1: <[AEF92] ACO 1682 N> (Nos 1-2), <[AEF92] ACO 1703 N> (Nos 1-2), <[AEF92] ACO 2219 N> (Nos 1-3)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AEGIS
AEGIS	(All-wavelength Extended Groth Strip International Survey)
*****	Avoid the usage of AEGIS, prefer [LNG2009]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: AEGIS20
AEGIS20	(All-wavelength Extended Groth strip International Survey 20cm data)
Write:	<<AEGIS20 JHHMMSS.ss+DDMMSS.s>>
N:	511 (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 20cm radio continuum observations of the Extended Groth strip.
in source:	NAME Extended Groth Strip
Ref:	=2012ApJ...756...72W
by	WILLNER S.P. , ASHBY M.L.N., BARMBY P., CHAPMAN S.C., COIL A.L., COOPER M.C., HUANG J.-S., IVISON R., KOO D.C.
	Astrophys. J., 756, 72 (2012)
	A fully identified sample of AEGIS20 microjansky radio sources.
o	Tables 1-5: <AEGIS20 JHHMMSS.ss+DDMMSS.s> N=511
=E=	Catalogue in electronic form as <J/ApJ/756/72/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AEGISXD
AEGISXD	(AEGIS-X Deep)
Write:	<<AEGISXD JHHMMSS.ss+DDMMSS.s>>
N:	937
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Catalog of N=937 X-ray sources detected in the deep (800ks) Chandra imaging of the AEGIS field. More information is available at http://www.mpe.mpg.de/XraySurveys See also [NLA2015].
in source:	NAME Extended Groth Strip
Ref:	=2015ApJS..220...10N
by	NANDRA K. , LAIRD E.S., AIRD J.A., SALVATO M., GEORGAKAKIS A., BARRO G., PEREZ-GONZALEZ P.G., BARMBY P., CHARY R.-R., COIL A., COOPER M.C., DAVIS M., DICKINSON M., FABER S.M., FAZIO G.G., GUHATHAKURTA P., GWYN S., HSU L.-T., HUANG J.-S., IVISON R.J., KOO D.C., NEWMAN J.A., RANGEL C., YAMADA T., WILLMER C.
	Astrophys. J., Suppl. Ser., 220, 10 (2015)
	AEGIS-X: Deep Chandra imaging of the central Groth Strip.
o	Table 11, col(1): <[NLA2015] aegis NNN> (Nos 1-937) = Table 11, col(2): <AEGISXD JHHMMSS.ss+DDMMSS.s> N=937.
=E=	Catalogue in electronic form as <J/ApJS/220/10/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AEL81]
[AEL81]	(Alloin+Edmunds+Linblad+, 1981)= (L)
Write:	<<[AEL81] LNNa>>
N:	14 among N>33
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
in source:	NGC 1365
Ref:	=1981A&A...101..377A
by	ALLOIN D. , EDMUNDS M.G., LINDBLAD P.O., PAGEL B.E.J.
	Astron. Astrophys., 101, 377-384 (1981)
	The mild abundance gradient of NGC 1365.
o	Complete list 'LNN' not found
o	Table 1: <[AEL81] LNNa> N=13 among (Nos L3 to L33, +L17d)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AEM97]
[AEM97]	(Ageorges+Eckart+Monin+, 2002)
Write:	<<[AEM97] AS 310 A>>
N:	6
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	SHARP 1/ESO-NTT observations. (NIR) image of AS 310: cluster of 6 sources.
in source:	NAME AS 310 Cluster
Ref:	=1997A&A...326..632A
by	AGEORGES N. , ECKART A., MONIN J.-L., MENARD F.
	Astron. Astrophys., 326, 632-639 (1997)
	New multiple young stellar objects discovered by near-infrared speckle imaging.
o	Table 1 : Hm 10 = Ass Cha T 1-10, 1548C27 = NIPSS 1548C27
o	Fig.7, Table 2: <[AEM97] AS 310 A> (Nos A-F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AER2001]
[AER2001]	(Alonso-Herrero+Engelbracht+Rieke+, 2001)
Write:	<<[AER2001] HII NN>> <<[AER2001] Cl NN>>
N:	13+16
Object:	HII + Cluster of * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST NICMOS observations of NGC 1614. Table 2: N=13 HII regions, (Nos 1-5) are ring HII regions, (Nos 6-13) are spiral arm HII regions. Table 4: N=16 star clusters.
in source:	NGC 1614
Ref:	=2001ApJ...546..952A
by	ALONSO-HERRERO A. , ENGELBRACHT C.W., RIEKE M.J., RIEKE G.H., QUILLEN A.C.
	Astrophys. J., 546, 952-965 (2001)
	NGC 1614: a laboratory for starburst evolution.
o	p. 953 : standard star P330-E = GSPC P330-E
o	Table 2: <[AER2001] HII NN> (Nos 1-13). Table 4: <[AER2001] Cl NN> (Nos 1-16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AER91]
[AER91]	(Anglada+Estalella+Rodriguez+, 1991)= (VLA)
Write:	<<[AER91] N>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	[AER91] 1 and 2 are found later in the literature as 'LDN 723 VLA 1' and '2'
in source:	LDN 723
Ref:	=1991ApJ...376..615A
by	ANGLADA G. , ESTALELLA R., RODRIGUEZ L.F., TORRELLES J.M., LOPEZ R., CANTO J.
	Astrophys. J., 376, 615-617 (1991)
	A double radio source at the center of the outflow in L 723.
o	[AER91] 1, 2 = NAME LDN 723 VLA 1, 2
o	Table 1: <[AER91] N> (Nos 1-3)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AES2005]
[AES2005]	(Asgekar+English+Safi-Harb+, 2005)
Write:	<<[AES2005] GLLL+B.b+VVV>> <<[AES2005] GLLL.l+B.b+VVV>>
N:	7
Object:	HI (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	Narrow vertical galactic HI structures found in the CGPS survey (INVS)
Ref:	=2005AJ....130..674A
by	ASGEKAR A. , ENGLISH J., SAFI-HARB S., KOTHES R.
	Astron. J., 130, 674-697 (2005)
	A search for narrow vertical structures in the Canadian Galactic plane survey.
o	Table 1: <INVS GLLL.l+B.b+VVV> N=10. Table 1: <[AES2005] GLLL+B.b+VVV>, <[AES2005] GLLL.l+B.b+VVV>, N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AES98]
[AES98]	(Arkhipova+Esipov+Sokol, 1998) (Not yet in Simbad)
Write:	<<[AES98] cN>> <<[AES98] a>>
N:	9+5
Object:	* (SIMBAD class: Star)
Note:	N=9 comparison stars (Nos c1-c9) in the field of FG Sge, and N=5 other stars (Nos k, l, n, x, y).
Ref:	=1998PAZh...24..431A
by	ARKHIPOVA V.P. , ESIPOV V.F., SOKOL G.V.
	Pis'ma Astron. Zh., 24, 431-437 (1998)
	UBV photometry and the spectrum of FG Sagittae in 1996-1997.
o	Fig.1, Table 2: <[AES98] cN> (Nos c1-c9), <[AES98] a> (Nos k, l, n, x, y).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AET95]
[AET95]	(Aschenbach+Egger+Trumper, 1995)
Write:	<<[AET95] A>> <<[AET95] A'>>
N:	6+1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT observations of the region around Vela SNR. (Nos A-F), N=6 features in the SNR, (No. D') west to feature D, looks like a diffuse arc.
in source:	NAME Vela SNR
Ref:	=1995Natur.373..587A
by	ASCHENBACH B. , EGGER R., TRUMPER J.
	Nature, 373, 587-589 (1995)
	Discovery of explosion fragments outside the Vela supernova remnant shock-wave boundary.
o	Fig.1: <[AET95] A> (Nos A-F), <[AET95] A'> (No. D').
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AF
AF	(A-F type *)
*****	Avoid the usage of AF, prefer Case A-F
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Af
Af	(Abell cl., faint)
*****	Avoid the usage of Af, prefer [CSD91]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AF
AF	(Air Force)
*****	Avoid the usage of AF, prefer RAFGL
Details on Acronym: [AF2011]
[AF2011]	(Azimlu+Fich, 2011)
Write:	<<[AF2011] SNNN CNN>> <<[AF2011] SNNN CNN-a>> <<[AF2011] SNNN-SNNN CNN>>
N:	142
Object:	Clump (SIMBAD class: denseCore = Dense Core)
Note:	JCMT 12CO(2-1) and 13CO(2-1) observations of HII regions.
Ref:	=2011AJ....141..123A
by	AZIMLU M. , FICH M.
	Astron. J., 141, 123 (2011)
	Study of molecular clouds associated with H II regions.
o	Tables 2-3: <[AF2011] SNNN CNN>, <[AF2011] SNNN-SNNN CNN> N=142.
=E=	Catalogue in electronic form as <J/AJ/141/123/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AFA2007]
[AFA2007]	(Auger+Fassnacht+Abrahamse+, 2007)
Write:	<<[AFA2007] JHHMMSS+DDMMSS>> <<[AFA2007] HHMM-N NN>>
N:	8+7+10+8
Object:	Group of G + G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Keck LRIS and ESI observations of the fields of CLASS 2319+051 and CLASS 1600+434. N=8 galaxy groups are found.
in source:	NAME B1600+434 GROUP
in source:	NAME B2319+051 FOREGROUND GROUP
in source:	NAME B2319+051 BACKGROUND GROUP
Ref:	=2007AJ....134..668A
by	AUGER M.W. , FASSNACHT C.D., ABRAHAMSE A.L., LUBIN L.M., SQUIRES G.K.
	Astron. J., 134, 668-679 (2007)
	The gravitational lens-galaxy group connection. II. Groups associated with B2319+051 and B1600+434.
o	Table 3: <[AFA2007] JHHMMSS+DDMMSS> N=8. Table 4: <[AFA2007] 1600-1 N> (Nos 1-7). Table 5: <[AFA2007] 2319-1 NN> (Nos 1-10).Table 6: <[AFA2007] 2319-2 N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AFCRL
AFCRL	(Air Force Cambridge Research Lab.)
Note:	updated by AFGL
====>	Equivalent to: RAFGL
Details on Acronym: [AFF2006]
[AFF2006]	(Antonello+Fossati+Fugazza+, 2006)= ([AFF2006a]) = (WFI)
Write:	<<[AFF2006] NNNN-N>>
N:	921
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Note:	BVRI observations collected with the WFI at the ESO 2.2 telescope at La Silla. In the format, the last digit stands for chip 1, 2, 3.
in source:	IC 1613
Ref:	=2006A&A...445..901A
by	ANTONELLO E. , FOSSATI L., FUGAZZA D., MANTEGAZZA L., GIEREN W.
	Astron. Astrophys., 445, 901-906 (2006)
	Variable stars in nearby galaxies. VII. P-L relation in the BVRI bands of Cepheids in IC 1613.
o	Fig.1 A0655 is a probable misprint for [AFM2000] V0555-A.
o	Table ic1613.dat: <[AFF2006] NNNN-N> N=921.
=E=	Catalogue in electronic form as J/A+A/445/901
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AFF2006a]
[AFF2006a]	(Antonello+Fossati+Fugazza+, 2006)
*****	Avoid the usage of [AFF2006a], prefer [AFF2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AFF2006b]
[AFF2006b]	(Argiroffi+Favata+Flaccomio+, 2006)
Write:	<<[AFF2006b] CTIO NNNN>> <<[AFF2006b] Danish NNNN>> <<[AFF2006b] XMM NNN>>
N:	5759+3570+224
Object:	* in Assoc. (SIMBAD class: Star)
Note:	XMM-Newton observations of young stars in 2 regions of the Upper Scorpius association. Additional optical observations at the CTIO Curtis Schmidt and Danish 1.54m telescopes.
in source:	NAME Upper Sco Assoc
Ref:	=2006A&A...459..199A
by	ARGIROFFI C. , FAVATA F., FLACCOMIO E., MAGGIO A., MICELA G., PERES G., SCIORTINO S.
	Astron. Astrophys., 459, 199-213 (2006)
	XMM-Newton survey of two upper Scorpius regions.
o	Table b1: <[AFF2006b] CTIO NNNN> (Nos 1-5759). Table c1: <[AFF2006b] Danish NNNN> (Nos 1-3570). Table d1: <[AFF2006b] XMM NNN> (Nos 1-224).
=E=	Catalogue in electronic form as J/A+A/459/199
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AFF2015]
[AFF2015]	(Alabi+Foster+Forbes+, 2015)
Write:	<<[AF2015] NGC4473 GCNNN>> <<[AF2015] NGC4473 starNN>> <<[AF2015] NGC4473 galNN>>
N:	106
Object:	GlCl + * + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST ACS, Subaru Suprime-Cam and Keck DEIMOS photometric and spectroscopic observations of N=106 globular clusters in NGC 4473 and N=? Galactic stars and background galaxies. In the formats, GC stands for spectroscopically confirmed GCs, star for spectroscopically confirmed Galactic stars and gal for background galaxies. See also [FSR2011], [PFR2013], [PBB2015] and [PFU2015].
in source:	NGC 4473
Ref:	=2015MNRAS.452.2208A
by	ALABI A.B. , FOSTER C., FORBES D.A., ROMANOWSKY A.J., PASTORELLO N., BRODIE J.P., SPITLER L.R., STRADER J., USHER C.
	Mon. Not. R. Astron. Soc., 452, 2208-2219 (2015)
	The SLUGGS survey: globular cluster kinematics in a `double σ' galaxy - NGC 4473.
o	Table 1: <[AFF2015] NGC4473 GCNNN> (Nos 1-106), <[AFF2015] NGC4473 starNN> N=?, <[AFF2015] NGC4473 galNN> N=?.
=E=	Catalogue in electronic form as J/MNRAS/452/2208
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AFG2011]
[AFG2011]	(Arellano Ferro+Figuera Jaimes+Giridhar+, 2011)
Write:	<<[AFG2011] SN>>
N:	5
Object:	Blue Straggler * (SIMBAD class: BlueStraggler = Blue Straggler)
Stat:	is completely incorporated in Simbad
Note:	Indian Astronomical Observatory (IAO) 2.0-m telescope (VI) observations of the globular cluster NGC 5024.
in source:	M 53 = NGC 5024
Ref:	=2011MNRAS.416.2265A
by	ARELLANO FERRO A. , FIGUERA JAIMES R., GIRIDHAR S., BRAMICH D.M., HERNANDEZ SANTISTEBAN J.V., KUPPUSWAMY K.
	Mon. Not. R. Astron. Soc., 416, 2265-2284 (2011)
	Exploring the variable stars in the globular cluster NGC 5024 (M53): new RR Lyrae and SX Phoenicis stars.
o	Fig. 2, Tables 2, 6: <Cl* NGC 5024 SAW VNNN> (Nos 91-105) added. Table 7: <[AFG2011] SN> (Nos S1-S5).
=E=	Catalogue in electronic form as J/MNRAS/416/2265
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AFGL
AFGL	(Air Force Geophys. Lab.)
====>	Equivalent to: RAFGL
Details on Acronym: [AFH2004]
[AFH2004]	(Alvarez+Feldt+Henning+, 2004)
Write:	<<[AFH2004] GLLL.ll+B.bb NNN>>
N:	99
Object:	* (SIMBAD class: Star)
Note:	Observations with ALFA and ADONIS AO systems at Calar Alto and La Silla Selected stars in 8 Ultra Compact HII regions.
in source:	GAL 309.92+00.48
in source:	GAL 351.16+00.70
in source:	GAL 005.88-00.41
in source:	GAL 011.11-00.40
in source:	GAL 018.15-00.28
in source:	GAL 061.48+00.09
in source:	GAL 070.29+01.60
in source:	GAL 077.96-00.01
Ref:	=2004ApJS..155..123A
by	ALVAREZ C. , FELDT M., HENNING T., PUGA E., BRANDNER W., STECKLUM B.
	Astrophys. J., Suppl. Ser., 155, 123-148 (2004)
	Near-infrared subarcsecond observations of ultracompact H II regions.
o	Table 3: <[AFH2004] GLLL.ll+B.bb NNN> N=99.
=E=	Catalogue in electronic form as J/ApJS/155/123
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AFH2012]
[AFH2012]	(Allevato+Finoguenov+Hasinger+, 2012)
Write:	<<[AFH2012] NNN>> <<[AFH2012] XMM NNNNN>> <<[AFH2012] Chandra NNNNN>>
N:	58+41+52
Object:	Group of G + AGN (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	X-ray emitting AGNs in galaxy groups based on COSMOS X-ray (XMM and Chandra) and optical data.
Ref:	=2012ApJ...758...47A
by	ALLEVATO V. , FINOGUENOV A., HASINGER G., MIYAJI T., CAPPELLUTI N., SALVATO M., ZAMORANI G., GILLI R., GEORGE M.R., TANAKA M., BRUSA M., SILVERMAN J., CIVANO F., ELVIS M., SHANKAR F.
	Astrophys. J., 758, 47 (2012)
	Occupation of x-ray-selected galaxy groups by X-ray active galactic nuclei.
o	Table 2: <[AFH2012] NNN> N=58 among (Nos 11-333), <[AFH2012] XMM NNNNN> N=41 among (Nos 6-60270), <[AFH2012] Chandra NNNNN> N=52 among (Nos 24-12390)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AFK2009]
[AFK2009]	(Aden+Feltzing+Koch+, 2009)= (INT) = ([AFK2009a])
Write:	<<[AFK2009] NNNNN>>
N:	58
Object:	* (SIMBAD class: Star)
Note:	INT WFC photometry and VLT FLAMES spectroscopy of stars in the Hercules dSph galaxy.
in source:	NAME Hercules Dwarf Galaxy
Ref:	=2009A&A...506.1147A
by	ADEN D. , FELTZING S., KOCH A., WILKINSON M.I., GREBEL E.K., LUNDSTROEM I., GILMORE G.F., ZUCKER D.B., BELOKUROV V., EVANS N.W., FARIA D.
	Astron. Astrophys., 506, 1147-1168 (2009)
	A photometric and spectroscopic study of the new dwarf spheroidal galaxy in Hercules . Metallicity, velocities, and a clean list of RGB members.
o	Tables 6, 7, 9: <[AFK2009] NNNNN> N=3+8+47 among (Nos 11239-43688).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AFK2009a]
[AFK2009a]	(Aden+Feltzing+Koch+, 2009)= (INT)
*****	Avoid the usage of [AFK2009a], prefer [AFK2009]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AFK2009b]
[AFK2009b]	(Anguita+Faure+Kneib+, 2009)
Write:	<<[AFK2009b] A>> <<[AFK2009b] JHHMMSS.ss+DDMMSS.s>>
N:	4+10
Object:	Grav. lensed image + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT FORS1 spectroscopy of objects in the field of COSMOS 5921+0638.
in source:	[FKC2008] COSMOS 5921+0638
Ref:	=2009A&A...507...35A
by	ANGUITA T. , FAURE C., KNEIB J.-P., WAMBSGANSS J., KNOBEL C., KOEKEMOER A.M., LIMOUSIN M.
	Astron. Astrophys., 507, 35-46 (2009)
	COSMOS 5921+0638: characterization and analysis of a new strong gravitationally lensed AGN.
o	Fig. 1: <[AFK2009b] A> (Nos A-D). Table 2, Fig. 3: <[AFK2009b] JHHMMSS.ss+DDMMSS.s> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AFK96]
[AFK96]	(Allen+Fabian+Kneib, 1996)
Write:	<<[AFK96] A>>
N:	3
Object:	Arc (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	CFHT image of PKS 0745-191. N=3 arcs, 'A' is the bright arc, B and C are fainter arc candidates.
Ref:	=1996MNRAS.279..615A
by	ALLEN S.W. , FABIAN A.C., KNEIB J.P.
	Mon. Not. R. Astron. Soc., 279, 615-635 (1996)
	A combined X-ray and gravitational lensing study of the massive cooling-flow cluster PKS 0745-191.
o	CCG = PGC 21813.
o	Fig.3: <[AFK96] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AFM2000]
[AFM2000]	(Antonello+Fugazza+Mantegazza, 2000)
Write:	<<[AFM2000] VNNNN-A>> <<[AFM2000] VaNNNN-A>>
Object:	Cepheid + V* (SIMBAD class: Variable* = Variable Star)
Note:	Observations of 4 fields (Nos A-D) in IC 1613. In the format 'VNNNN-A' the letter 'A' stands for the fields, 'Va' stands for two stars in the same field with the same number, ex.: Va2942-B is a Ce, Vb2942-B is a V. In field A, numbering is the same as in [AMF99] VNNNN. See also [AFM2002], [AFM2002b].
in source:	IC 1613
Ref:	=2000A&A...356L..37A
by	ANTONELLO E. , FUGAZZA D., MANTEGAZZA L.
	Astron. Astrophys., 356, 37-40 (2000)
	Metallicity effects on the light curve shape of Cepheids with period close to 10 days.
o	Table 1: <[AFM2000] VNNNN-A> N=16.
Ref:	=2000A&A...363...29A
by	ANTONELLO E. , FUGAZZA D., MANTEGAZZA L., BOSSI M., COVINO S.
	Astron. Astrophys., 363, 29-40 (2000)
	Variable stars in nearby galaxies. III. White light observations of Field B of IC 1613.
o	Tables 8, 9: <[AFM2000] VNNNN-B> N=51+70 (115 are new), <[AFM2000] VaNNNN-B> N=2.
Ref:	=2001A&A...367..759M
by	MANTEGAZZA L. , ANTONELLO E., FUGAZZA D., BOSSI M., COVINO S.
	Astron. Astrophys., 367, 759-769 (2001)
	Variable stars in nearby galaxies. IV. Fields C and D of IC 1613.
o	Tables 3, 4: <[AFM2000] VNNNN-C> N=13+39, <[AFM2000] VNNNN-D> N=2+19.
=E=	Catalogue in electronic form as J/A+A/363/29
=E=	Catalogue in electronic form as J/A+A/367/759
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AFM2002]
[AFM2002]	(Antonello+Fugazza+Mantegazza, 2002)= ([AFM2002a])
Write:	<<[AFM2002] FFa-NNNN>>
N:	69+10
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Stat:	is completely incorporated in Simbad
Note:	CCD observations of Cepheids in the SMC. N=69 Cepheids + 10 candidates.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2002A&A...385..793A
by	ANTONELLO E. , FUGAZZA D., MANTEGAZZA L.
	Astron. Astrophys., 385, 793-801 (2002)
	Search for second overtone mode Cepheids in Magellanic Clouds. II. Characteristics of second overtone mode pulsations.
o	Tables 3, 4, 5: <[AFM2002] FFa-NNNN> N=69+10.
=E=	Catalogue in electronic form as J/A+A/385/793
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AFM2002a]
[AFM2002a]	(Antonello+Fugazza+Mantegazza, 2002)
Note:	See also [AMF99], [AFM2000], [AFM2002b].
*****	Avoid the usage of [AFM2002a], prefer [AFM2002]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AFM2002b]
[AFM2002b]	(Antonello+Fugazza+Mantegazza, 2002)
Write:	<<[AFM2002b] VNNNN>>
N:	130
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	See also [AMF99], [AFM2000], [AFM2002].
in source:	NGC 6822
Ref:	=2002A&A...386..860A
by	ANTONELLO E. , FUGAZZA D., MANTEGAZZA L., STEFANON M., COVINO S.
	Astron. Astrophys., 386, 860-864 (2002)
	Variable stars in nearby galaxies. V. Search for Cepheids in field A of NGC 6822.
o	in ref list MADORE 1991PASP..103..933M instead of 103.993
o	Fig.1, Table 1: <[AFM2002b] VNNNN> N=130 among (Nos V3-V3984).
Ref:	=2002IBVS.5254....1A
by	ANTONELLO E. , FUGAZZA D., MANTEGAZZA L., STEFANON M.
	IAU Inform. Bull. Var. Stars, 5254, 1-None (2002)
	Variable stars in field a of NGC 6822.
o	Tables 1, 2: <[AFM2002b] VNNNN> N=13+91 among (Nos V2-V4443).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AFM2007]
[AFM2007]	(Albacete Colombo+Flaccomio+Micela+, 2007)
Write:	<<[AFM2007] NNNN>>
N:	1003
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Analysis of Chandra ACIS-I observations of the core of the Cygnus OB2 region. See also CXOCyg
in source:	Ass Cyg OB 2 = NAME VI CYG
Ref:	=2007A&A...464..211A
by	ALBACETE COLOMBO J.F. , FLACCOMIO E., MICELA G., SCIORTINO S., DAMIANI F.
	Astron. Astrophys., 464, 211-227 (2007)
	Unveiling the Cygnus OB2 stellar population with Chandra.
o	Table 1, col(1): <[AFM2007] NNNN> (Nos 1-1003) = Table 1, col(2): <CXOCyg JHHMMSS.ss+DDMMSS.s> N=1003.
=E=	Catalogue in electronic form as J/A+A/464/211
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AFM2009]
[AFM2009]	(Azimlu+Fich+McCoey, 2009)
Write:	<<[AFM2009] S175A>> <<[AFM2009] S175A CNN>>
N:	3+13+12
Object:	MCld + Clump (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	JCMT 12CO(2-1) observations of S175.
in source:	SH 2-175
Ref:	=2009AJ....137.4897A
by	AZIMLU M. , FICH M., McCOEY C.
	Astron. J., 137, 4897-4910 (2009)
	Studies of molecular clouds associated with H II regions: S175.
o	Text: <[AFM2009] S175A> (Nos S175A-S175C). Tables 1, 2: <[AFM2009] S175A CNN> (Nos S175A C1-C13, S175B C1-C12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AFN2013]
[AFN2013]	(Armstrong+Fender+Nicolson+, 2013) (Not yet in Simbad)
Write:	<<[AFN2013] WW>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	MeerKAT test array KAT-7 observations at 1.9GHz of Circinus X-1.
Ref:	=2013MNRAS.433.1951A
by	ARMSTRONG R.P. , FENDER R.P., NICOLSON G.D., RATCLIFFE S., LINARES M., HORRELL J., RICHTER L., SCHURCH M.P.E., CORIAT M., WOUDT P., JONAS J., BOOTH R., FANAROFF B.
	Mon. Not. R. Astron. Soc., 433, 1951-1957 (2013)
	A return to strong radio flaring by Circinus X-1 observed with the Karoo Array Telescope test array KAT-7.
o	Fig. 1: <[AFN2013] WW> (Nos NE, NW).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AFO2003]
[AFO2003]	(Arnaboldi+Freeman+Okamura+, 2003)
Write:	<<[AFO2003] NNNN>> <<[AFO2003] AAN>>
N:	10+3
Object:	Poss. PN (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
Note:	Subaru observations, TNG and VLT confirmations. Candidates for Intra Cluster PN (ICPN) in Virgo cluster. Format 10NN for objects in the outer region of M 84. Format IC1 to IC3 for objects in the authors IC field. See also [OYA2002].
in source:	NAME Virgo Cluster
Ref:	=2003AJ....125..514A
by	ARNABOLDI M. , FREEMAN K.C., OKAMURA S., YASUDA N., GERHARD O., NAPOLITANO N.R., PANNELLA M., ANDO H., DOI M., FURUSAWA H., HAMABE M., KIMURA M., KAJINO T., KOMIYAMA Y., MIYAZAKI S., NAKATA F., OUCHI M., SEKIGUCHI M., SHIMASAKU K., YAGI M.
	Astron. J., 125, 514-524 (2003)
	Narrowband imaging in [O III] and Hα to search for intracluster planetary nebulae in the Virgo cluster.
o	Table 2: <[AFO2003] 10NN> N=10 among (Nos 103 and 1017). Table 3: <[AFO2003] ICN> (Nos IC1-IC3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AFR2020]
[AFR2020]	(Alabi+Forbes+Romanowsky+, 2020)
Write:	<<[AFR2020] NGC5907 GCNNN>> <<[AFR2020] NGC5907 YCNN>> <<[AFR2020] NGC5907 StarNN>> <<[AFR2020] NGC5907 GalN>>
N:	315+34+64+7
Object:	Poss. GlCl + Poss. Young Cluster of * + * + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Subaru Suprime-Cam imaging and Keck II DEIMOS spectroscopy of N=315 globular cluster candidates ({GC}), N=34 young star cluster candidates, N=64 Milky Way stars, and N=7 background galaxies in the field of NGC 5907.
in source:	NGC 5907
Ref:	=2020MNRAS.491.5693A
by	ALABI A.B. , FORBES D.A., ROMANOWSKY A.J., BRODIE J.P.
	Mon. Not. R. Astron. Soc., 491, 5693-5701 (2020)
	Globular clusters in the stellar stream surrounding the Milky Way analogue NGC 5907.
o	Table 2: <[AFR2020] NGC 5907 GCNNN> (Nos GC1-GC315), <[AFR2020] NGC 5907 YCNNN> (Nos YC1-YC33, YC43), <[AFR2020] NGC 5907 StarNNN> (Nos Star1-Star64), <[AFR2020] NGC 5907 GalN> (Nos Gal1-Gal7).
=E=	Catalogue in electronic form as <J/MNRAS/491/5693/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [AFW2008]
[AFW2008]	(Auger Fassnacht+Wong+, 2008)
Write:	<<[AFW2008] JHHMMSS.ss+DDMMSS.s>> <<[AFW2008] JHHMMSS.sss+DDMMSS.ss>>
N:	3+5+13+10
Object:	Group of G + G in Group of G (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Keck NIRC2 AO imaging and Keck ESI spectroscopy of the field of SBSG 1520+530.
Ref:	=2008ApJ...673..778A
by	AUGER M.W. , FASSNACHT C.D., WONG K.C., THOMPSON D., MATTHEWS K., SOIFER B.T.
	Astrophys. J., 673, 778-786 (2008)
	Lens galaxy properties of SBS 1520+530: insights from Keck spectroscopy and AO imaging.
o	Table 4: <[AFW2008] JHHMMSS.ss+DDMMSS.s> N=3. Table 5: <[AFW2008] JHHMMSS.sss+DDMMSS.ss> N=5+13+10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AG
AG	(Arce+Goodman) (Not yet in Simbad)
*****	Avoid the usage of AG, prefer [AG99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AG
AG	(Astr. Gesellschaft katalog)= AGK = AGK2 = (AGK/2) = AGK3 = (AGK/3) = (AGK3U)
Write:	<<AG +DD NNNN>> <<AG +DD NNNN.N>>
N:	170464
Object:	* (SIMBAD class: Star)
Note:	The first AGK and second AGK2 editions are superseded by AGK3 Star Catalogue of positions and proper motions north of -2.5deg declination 1992AJ....103.1689B is an updated version of the AGK3. The AGK3 proper motions are improved, using the Palomar 'Quick V' survey, reaching a formal mean error 0.82"/century. The AGK3U positions have a mean error of 0.167" at an average epoch of 1950.62.
Ref:	=1975AGK3..C......0H
by	HECKMANN O. , DIECKVOSS W.
	AGK3 Catalogue, 0-None (1975)
	AGK3 : star catalogue of positions and proper motions, north of 2 .5 declination : derived from photographic plates taken at Bergedorf and Bonn in the years 1928-1932 and 1956-1963.
o	<AG+DD NNNN>, <AG+DD NNNN.n>, N=180000.
Ref:	=1992AJ....103.1689B
by	BUCCIARELLI B. , DAOU D., LATTANZI M.G., TAFF L.G.
	Astron. J., 103, 1689-None (1992)
	The AGK3 U: an updated version of the AGK3.
o	<AG+DD NNNN> N=170464.
=E=	Catalogue in electronic form as I/176
=E=	Catalogue in electronic form as I/61
Origin	of the Acronym: L = Found in the literature
Details on Acronym: AG
AG	(Allen+Goss)
*****	Avoid the usage of AG, prefer [AG79]
Origin	of the Acronym: L (1984ApJ...277..542H)
Details on Acronym: AG
AG	(Anticenter Galactic)
*****	Avoid the usage of AG, prefer [GB2001]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AG2001]
[AG2001]	(Arce+Goodman, 2001) (Not yet in Simbad)
Write:	<<[AG2001] RN>>
N:	5
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Note:	N=5 outflow clumps in the region associated with the HH 300 flow from the young star IRAS 04239+2436.
in source:	HH 300
Ref:	=2001ApJ...554..132A
by	ARCE H.G. , GOODMAN A.A.
	Astrophys. J., 554, 132-151 (2001)
	The episodic, precessing giant molecular outflow from IRAS 04239+2436 (HH 300).
o	Barn 18w = [WMD94] Tau G 1
o	Table 1, Figs 4, 5: <[AG2001] RN> (Nos R1-R5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AG79]
[AG79]	(Allen+Goss, 1979)= (AG)
Write:	<<[AG79] NN>>
N:	11
Object:	Star (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=11 stars in the field of M 101
in source:	M 101 = NGC 5457
Ref:	=1979A&AS...36..135A
by	ALLEN R.J. , GOSS W.M.
	Astron. Astrophys., Suppl. Ser., 36, 135-162 (1979)
	The giant spiral galaxy M 101. V. A complete synthesis of the distribution and motions of the neutral hydrogen.
o	Table 2: <[AG79] NN> (Nos 1-11)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AG82
AG82	(Acker+Gleizes+, 1982)= (FC)
Write:	<<AG82 NNN>> <<AG82 NNNbis>>
N:	460
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	3 Complements and Errata have been published in 1982, 1983, 1984 at 'Edit. Obs. of Strasbourg' In 1984, N=13 new objects have a format 'NNNbis' (not used)
Ref:	=1982PSCDS...3....0A
by	ACKER A. , GLEIZES F., CHOPINET M., MARCOUT J., OCHSENBEIN F., ROQUES J.M.
	Publ. Speciale C.D.S., -1-None (1982)
	Catalogue of the central stars of true and possible planetary nebulae.
o	<AG82 NNN> N=460
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [AG92]
[AG92]	(Arnold+Gilmore, 1992)= (BHB)
Write:	<<[AG92] NNNNN>>
N:	44
Object:	Blue HB* (SIMBAD class: HorBranch* = Horizontal Branch Star)
Stat:	is completely incorporated in Simbad
Note:	N=44 BHB selected from digitized UK Schmidt plates.
Ref:	=1992MNRAS.257..225A
by	ARNOLD R. , GILMORE G.
	Mon. Not. R. Astron. Soc., 257, 225-239 (1992)
	Halo blue horizontal branch stars: spectroscopy in two fields.
o	Tables 1, 2: <[AG92] NNNNN> N=44
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AG99]
[AG99]	(Arce+Goodman, 1999)= (AG) = [AG99a] = (TDC) (Not yet in Simbad)
Write:	<<[AG99] NNNNNN>> <<[AG99] TDC NNN>> <<[AG99] AG NNN>> <<[AG99] NNAN.N>> <<[AG99] NNAaN>> <<[AG99] NANN.N>> <<[AG99] ANN.NN>>
N:	62+16+5+10
Object:	* (SIMBAD class: Star)
in source:	NAME Tau Dark Cloud
Ref:	=1999ApJ...517..264A
by	ARCE H.G. , GOODMAN A.A.
	Astrophys. J., 517, 264-281 (1999)
	An extinction study of the Taurus dark cloud complex.
o	Table 1: stars are not in SIMBAD.
o	Table 1: <[AG99] NNNNNN> N=62, <[AG99] TDC NNN> N=16, <[AG99] AG NNN> N=5, <[AG99] NNAN.N>, <[AG99] NNAaN>, <[AG99] NANN.N>, <[AG99] ANN.NN> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AG99a]
[AG99a]	(Arce+Goodman, 1999) (Not yet in Simbad)
*****	Avoid the usage of [AG99a], prefer [AG99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AG99b]
[AG99b]	(Astier+Goobar, 1999)
Write:	<<[AG99b] JHHMMSS.ss+DDMMSS.s>>
N:	10
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxies of SN 1999DR to SN 1999EA.
Ref:	=1999IAUC.7258Q...1A
by	ASTIER P. , GOOBAR A.
	IAU Circ., 7258, 1-None (1999)
	Supernovae.
o	<[AG99b] JHHMMSS.ss+DDMMSS.s> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AGAL
AGAL	(ATLASGAL)= (ATLASGAL)
Write:	<<AGAL GLLL.lll+BB.bbb>> <<AGAL LLL.lll+BB.bbb>> (not recognised by Simbad, but found in literature)
N:	10163
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	ATLASGAL is the APEX Telescope Large Area Survey of the Galaxy, an observing programme with the LABOCA bolometer array at APEX (on Chajnantor, Chile). This survey mapped over 400 square degrees at 870 microns in the inner Galaxy, with a uniform sensitivity of a few solar masses at 1kpc distance. http://www3.mpifr-bonn.mpg.de/div/atlasgal/ 2013A&A...549A..45C: ATLASGAL compact source catalog (N=6639), first reference with AGAL objects. 2014A&A...568A..41U: ATLASGAL complete compact source catalog (N=10163).
Ref:	=2013A&A...549A..45C
by	CONTRERAS Y. , SCHULLER F., URQUHART J.S., CSENGERI T., WYROWSKI F., BEUTHER H., BONTEMPS S., BRONFMAN L., HENNING T., MENTEN K.M., SCHILKE P., WALMSLEY C.M., WIENEN M., TACKENBERG J., LINZ H.
	Astron. Astrophys., 549A, 45-45 (2013)
	ATLASGAL - compact source catalogue: 330° <l< 21°.
o	atl-csc: <AGAL GLLL.lll+BB.bbb> N=6639.
Ref:	=2014A&A...568A..41U
by	URQUHART J.S. , CSENGERI T., WYROWSKI F., SCHULLER F., BONTEMPS S., BRONFMAN L., MENTEN K.M., WALMSLEY C.M., CONTRERAS Y., BEUTHER H., WIENEN M., LINZ H.
	Astron. Astrophys., 568A, 41-41 (2014)
	ATLASGAL - Complete compact source catalogue: 280° <l< 60°.
o	atl-csc: <AGAL GLLL.lll+BB.bbb> N=10163.
=E=	Catalogue in electronic form as J/A+A/549/A45
=E=	Catalogue in electronic form as J/A+A/568/A41
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AGAPE
AGAPE	(Andromeda Galaxy, Amplified Pixel Experiment)
Write:	<<AGAPE ZNN>>
N:	1
Object:	Lensing Event (SIMBAD class: LensingEv = (Micro)Lensing Event)
Note:	See also AGAPE variable stars.
in source:	M 31 = NGC 224
Ref:	=1999A&A...344L..49A
by	ANSARI R. , AURIERE M., BAILLON P., BOUQUET A., COUPINOT G., COUTURES C., GHESQUIERE C., GIRAUD-HERAUD Y., GONDOLO P., HECQUET J., KAPLAN J., KIM A., LE DU Y., MELCHIOR A.L., MONIEZ M., PICAT J.P., SOUCAIL G.
	Astron. Astrophys., 344, 49-52 (1999)
	AgapeZ1: a large amplification microlensing event or an odd variable star towards the inner bulge of M31.
o	<AGAPE Z1> N=1.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AGAPE
AGAPE	(Andromeda Galaxy, Amplified Pixel Experiment)= (AGPV) = (AGP)
Write:	<<AGAPE VNNNN>> <<AGAPE NOVNN>>
N:	1579
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	AGAPE catalogue of variable stars. N=1579 V*, with format 'VNNNN', among which 12 are novae format 'NOVNN'. See also AGAPE lensing events.
in source:	M 31 = NGC 224
Ref:	=2004A&A...421..509A
by	ANSARI R. , AURIERE M., BAILLON P., BOUQUET A., COUPINOT G., COUTURES C., GHESQUIERE C., GIRAUD-HERAUD Y., GILLIERON D., GONDOLO P., HECQUET J., KAPLAN J., KIM A., LE DU Y., MELCHIOR A.L., MONIEZ M., PICAT J.P., SOUCAIL G.
	Astron. Astrophys., 421, 509-518 (2004)
	Variable stars towards the bulge of M 31: The AGAPE catalogue.
o	Table 3: format ANNN in col(2) is not used in SIMBAD (AGAPE Z1 is not AGAPE V1578: Author AURIERE M.). Par. 4.2, V38 probable misprint for V8 (BASW 8 in SIMBAD)
o	Table 3: <AGAPE VNNNN> (Nos V1-V1579). Table 4: <AGAPE NOVNN> (Nos NOV01 to NOV12).
=E=	Catalogue in electronic form as J/A+A/421/509
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AGAPE
AGAPE	(Andromeda Galaxy, Amplified Pixel Experiment)
Note:	AGAPE candidate events toward M 31.
*****	Avoid the usage of AGAPE, prefer [CDD2000b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AGASC
AGASC	(AXAF Guide and Acquisition Star Catalog)
Write:	<<AGASC NNNNNNNNNN>>
N:	18865968
Object:	* (SIMBAD class: Star)
Note:	All-sky astrometric and photometric catalog prepared for the operation of Chandra (formerly AXAF). The catalogue is described in Schmidt & Green (2003ASPC..295...81S), and available at the following website: http://www.astronomy.csdb.cn/asc/cgi-gen/cda/agasc/agascInterface.pl.htm
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AGC
AGC	(A.G. Clark)
Write:	<<** AGC NN>>
N:	15
Object:	(SIMBAD class: = Double or Multiple Star)
Auth.:	CLARK A.G.
Details on Acronym: AGC
AGC	(Arecibo General Catalog)= (A)
Write:	<<AGC NNNNNNA>>
Object:	G (SIMBAD class: Galaxy)
Note:	Internal coding number used by the authors, from their private database, referred to as the Arecibo General Catalog. Northern Hemisphere: Numbers 1 to 12943: Galaxies in UGC are assigned UGC numbers. The few noted in the UGC addenda receive sequential numbers above 12921 (original maximum UGC designation) Numbers above 100000: Additional entries in UGC. Assignment made on basis of hours of R.A. when number assignment is made (i.e. number is not changed if position update moves object to different R.A. hour). 100001-110000: 0-1h north, 110001-120000: 1-2h north, etc. Southern Hemisphere: Numbers 20001 to 36562: Assignment sequentially performed on original digital catalog of entries in ESO-Uppsala catalog. Unfortunately, digital version had some errors, so this assignment is not perfect. Numbers above 400000 : Additional assignment performed similarly to north, based on assignment per hour of R.A., 400001-409999: 0-1h south, 410001-420000: 1-2h south See also [SSG95]. Only the N=3 first references containing AGC lists are cited.
Ref:	=1995ApJ...444...41S
by	SCODEGGIO M. , SOLANES J.M., GIOVANELLI R., HAYNES M.P.
	Astrophys. J., 444, 41-63 (1995)
	The spatial distribution, kinematics, and dynamics of the galaxies in the region of Abell 2634 and 2666.
o	table 4 : CL 37 = RX J233756.1+271131
o	Tables 1, 2, 3: <[SSG95] NNNNNNA> = <AGC NNNNNNA> N=122.
Ref:	=1997AJ....113...22G
by	GIOVANELLI R. , HAYNES M.P., HERTER T., VOGT N.P., WEGNER G., SALZER J.J., DA COSTA L.N., FREUDLING W.
	Astron. J., 113, 22-52 (1997)
	The I band Tully-Fisher relation for cluster galaxies: data presentation.
o	Table 1: ESO 508 = NAME ESO 508. Table 2: N=782, 486 AGC and 296 UGC objects.
o	Table 2: <AGC NNNNNN> N=486 among (Nos 21943-530085).
Ref:	=1997AJ....113.1197H
by	HAYNES M.P. , GIOVANELLI R., HERTER T., VOGT N.P., FREUDLING W., MAIA M.A.G., SALZER J.J., WEGNER G.
	Astron. J., 113, 1197-1211 (1997)
	21 cm H I line spectra of galaxies in nearby clusters.
o	Tables 2, 3: <AGC NNNNNN> N=359+214.
=E=	Catalogue in electronic form as J/AJ/113/22
=E=	Catalogue in electronic form as J/AJ/113/1197
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AGC2010]
[AGC2010]	(Andrews+Gallagher+Clayton+, 2010) (Not yet in Simbad)
Write:	<<[AGC2010] A>>
N:	5
Object:	* (SIMBAD class: Star)
Note:	Observations of N=5 tertiary standards for UGC 12846, with the CTIO Yale 1.0m telescope.
Ref:	=2010ApJ...715..541A
by	ANDREWS J.E. , GALLAGHER J.S., CLAYTON G.C., SUGERMAN B.E.K., CHATELAIN J.P., CLEM J., WELCH D.L., BARLOW M.J., ERCOLANO B., FABBRI J., WESSON R., MEIXNER M.
	Astrophys. J., 715, 541-549 (2010)
	SN 2007od: a type IIP supernova with circumstellar interaction.
o	Fig. 1, Table 6: <[AGC2010] A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AGC2011]
[AGC2011]	(Amanullah+Goobar+Clement+, 2011)
Write:	<<[AGC2011] SN>>
N:	1
Object:	SN (SIMBAD class: Supernova = SuperNova)
Note:	VLT HAWK-I and NOT ALFOSC observations of a supernovae at redshift z=1.703 behind the massive cluster Abell 1689.
in source:	ACO 1689
Ref:	=2011ApJ...742L...7A
by	AMANULLAH R. , GOOBAR A., CLEMENT B., CUBY J.-G., DAHLE H., DAHLEN T., HJORTH J., FABBRO S., JONSSON J., KNEIB J.-P., LIDMAN C., LIMOUSIN M., MILVANG-JENSEN B., MORTSELL E., NORDIN J., PAECH K., RICHARD J., RIEHM T., STANISHEV V., WATSON D.
	Astrophys. J., 742L, 7 (2011)
	A highly magnified supernova at z = 1.703 behind the massive galaxy cluster A1689.
o	Fig. 1: <[AGC2011] SN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AGEL
AGEL	(ASTRO 3D Galaxy Evolution with Lenses)
Write:	<<AGEL JHHMMSS+DDMMSS system>> <<AGEL JHHMMSS+DDMMSS lens>> <<AGEL JHHMMSS+DDMMSS source>> <<AGEL HHMMSS+DDMMSS>> (not recognised by Simbad, but found in literature)
N:	79+68+68
Object:	Poss. Grav. lens system + Grav. lens + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Keck (ESI and NIRES) and VLT (X-Shooter) observations of N=68 gravitational lenses and N=68 background sources in N=79 gravitational lens system candidates, as part of our ASTRO 3D Galaxy Evolution with Lenses (AGEL) survey. Use of SLACS, BELLS, CASSOWARY, and DESI Legacy Imaging Survey data.
Ref:	=2022AJ....164..148T
by	TRAN K.-V.H. , HARSHAN A., GLAZEBROOK K., KEERTHI VASAN G.C., JONES T., JACOBS C., KACPRZAK G.G., BARONE T.M., COLLETT T.E., GUPTA A., HENDERSON A., KEWLEY L.J., LOPEZ S., NANAYAKKARA T., SANDERS R.L., SWEET S.M.
	Astron. J., 164, 148 (2022)
	The AGEL Survey: Spectroscopic Confirmation of Strong Gravitational Lenses in the DES and DECaLS Fields Selected Using Convolutional Neural Networks.
o	Fig. 2, Table 2: <AGEL JHHMMSS+DDMMSS system> N=79, <AGEL JHHMMSS+DDMMSS lens> N=68, <AGEL JHHMMSS+DDMMSS source> N=68.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AGES
AGES	(Arecibo Galaxy Environment Survey)
Write:	<<AGES JHHMMSS+DDMMSS>>
N:	22+100+87
Object:	HI (SIMBAD class: HI = HI (21cm) Source)
Note:	Arecibo Galaxy Environment Survey. Description of the survey and N=22 precursor observations in 2006MNRAS.371.1617A.
Ref:	=2006MNRAS.371.1617A
by	AULD R. , MINCHIN R.F., DAVIES J.I., CATINELLA B., VAN DRIEL W., HENNING P.A., LINDER S., MOMJIAN E., MULLER E., O'NEIL K., SABATINI S., SCHNEIDER S., BOTHUN G., CORTESE L., DISNEY M., HOFFMAN G.L., PUTMAN M., ROSENBERG J.L., BAES M., DE BLOK W.J.G., BOSELLI A., BRINKS E., BROSCH N., IRWIN J., KARACHENTSEV I.D., KILBORN V.A., KORIBALSKI B., SPEKKENS K.
	Mon. Not. R. Astron. Soc., 371, 1617-1640 (2006)
	The Arecibo Galaxy Environment Survey: precursor observations of the NGC 628 group.
o	Table 3: <AGES JHHMMSS+DDMMSS> N=22.
Ref:	=2008MNRAS.383.1519C
by	CORTESE L. , MINCHIN R.F., AULD R.R., DAVIES J.I., CATINELLA B., MOMJIAN E., ROSENBERG J.L., TAYLOR R., GAVAZZI G., O'NEIL K., BAES M., BOSELLI A., BOTHUN G., KORIBALSKI B., SCHNEIDER S., VAN DRIEL W.
	Mon. Not. R. Astron. Soc., 383, 1519-1537 (2008)
	The Arecibo Galaxy Environment Survey - II. A HI view of the Abell cluster 1367 and its outskirts.
o	Table 1: <AGES JHHMMSS+DDMMSS> N=100.
Ref:	=2010AJ....140.1093M
by	MINCHIN R.F. , MOMJIAN E., AULD R., DAVIES J.I., VALLS-GABAUD D., KARACHENTSEV I.D., HENNING P.A., O'NEIL K.L., SCHNEIDER S., SMITH M.W.L., STAGE M.D., TAYLOR R., VAN DRIEL W.
	Astron. J., 140, 1093-1118 (2010)
	The Arecibo Galaxy Environment Survey. III. Observations toward the galaxy pair NGC 7332/7339 and the isolated galaxy NGC 1156.
o	Table 1: <AGES JHHMMSS+DDMMSS> N=87.
=E=	Catalogue in electronic form as J/MNRAS/383/1519
=E=	Catalogue in electronic form as J/AJ/140/1093
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AGF2015]
[AGF2015]	(Anderson+Gaensler+Feain+, 2015) (Not yet in Simbad)
Write:	<<[AGF2015] JHHMMSS+DDMMSS>>
N:	160
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ATCA observations of N=160 polarized radio sources.
Ref:	=2015ApJ...815...49A
by	ANDERSON C.S. , GAENSLER B.M., FEAIN I.J., FRANZEN T.M.O.
	Astrophys. J., 815, 49 (2015)
	Broadband radio polarimetry and Faraday rotation of 563 extragalactic radio sources.
o	(Erratum) erratum vol. 820, art. 144 (2016)
o	Table 1: <[AGF2015] JHHMMSS+DDMMSS> N=160.
=E=	Catalogue in electronic form as <J/ApJ/815/49/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AGG2006]
[AGG2006]	(Akylas+Georgantopoulos+Georgakakis+, 2006)
Write:	<<[AGG2006] NNN>>
N:	153
Object:	AGN (SIMBAD class: AGN = Active Galaxy Nucleus)
Note:	XMM-Newton and Chandra observations of SDSS QSOs.
Ref:	=2006A&A...459..693A
by	AKYLAS A. , GEORGANTOPOULOS I., GEORGAKAKIS A., KITSIONAS S., HATZIMINAOGLOU E.
	Astron. Astrophys., 459, 693-701 (2006)
	XMM-Newton and Chandra measurements of the AGN intrinsic absorption: dependence on luminosity and redshift.
o	Table 2: <[AGG2006] NNN> (Nos 1-153).
=E=	Catalogue in electronic form as J/A+A/459/693
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AGJ2018]
[AGJ2018]	(Agnello+Grillo+Jones+, 2018)
Write:	<<[AGJ2018] SDSS J1433+6007 system>> <<[AGJ2018] SDSS J1433+6007 source>> <<[AGJ2018] SDSS J1433+6007 A>>
N:	1+1+5
Object:	Grav. lens system + QSO + Grav. lensed image of a QSO + Grav. lens (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	NOT ALFOSC and Keck II ESI observations of N=1 gravitational lens system, comprising N=1 background QSO, N=4 gravitationally lensed images of the QSO, and N=1 gravitational lens. Use of SDSS DR12 data.
Ref:	=2018MNRAS.474.3391A
by	AGNELLO A. , GRILLO C., JONES T., TREU T., BONAMIGO M., SUYU S.H.
	Mon. Not. R. Astron. Soc., 474, 3391-3396 (2018)
	Discovery and first models of the quadruply lensed quasar SDSS J1433+6007.
o	Fig. 1, Table 1: <[AGJ2018] SDSS J1433+6007 system> N=1, <[AGJ2018] SDSS J1433+6007 source> N=1, <[AGJ2018] SDSS J1433+6007 A> (Nos A-D, G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AGK
AGK	(Astr. Gesellschaft Katalog)
Note:	Superseded by AGK3
====>	Equivalent to: AG
Details on Acronym: AGK/2
AGK/2	(Astr. Gesellschaft Katalog, 2nd version)
Note:	Superseded by AGK3
*****	Avoid the usage of AGK/2, prefer AG
Details on Acronym: AGK/3
AGK/3	(Astr. Gesellschaft Katalog, 3rd version)
*****	Avoid the usage of AGK/3, prefer AG
Details on Acronym: AGK2
AGK2	(Astr. Gesellschaft Katalog, 2nd version)
Note:	Superseded by AGK3
====>	Equivalent to: AG
Details on Acronym: [AGK2007]
[AGK2007]	(Ardila+Golimowski+Krist+, 2007)
Write:	<<[AGK2007] N>>
N:	9
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	HST ACS coronographic observations of HD 100546 field.
Ref:	=2007ApJ...665..512A
by	ARDILA D.R. , GOLIMOWSKI D.A., KRIST J.E., CLAMPIN M., FORD H.C., ILLINGWORTH G.D.
	Astrophys. J., 665, 512-534 (2007)
	Hubble Space Telescope advanced camera for surveys coronagraphic observations of the dust surrounding HD 100546.
o	Table 3: <[AGK2007] N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AGK2012]
[AGK2012]	(Allen+Gutermuth+Kryukova+, 2012)
Write:	<<[AGK2012] JHHMMSS.ss+DDMMSS.s>> <<[AGK2012] Cep OB3b East>> <<[AGK2012] Cep OB3b West>>
N:	2575+1+1
Object:	YSO + Cluster of * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC and MIPS and Chandra ACIS observations of a rich massive young cluster in the Cep OB3b association.
in source:	NAME Ass Cep OB 3b
Ref:	=2012ApJ...750..125A
by	ALLEN T.S. , GUTERMUTH R.A., KRYUKOVA E., MEGEATH S.T., PIPHER J.L., NAYLOR T., JEFFRIES R.D., WOLK S.J., SPITZBART B., MUZEROLLE J.
	Astrophys. J., 750, 125 (2012)
	Spitzer imaging of the nearby rich young cluster, Cep OB3b.
o	Tables 1-4: <[AGK2012] JHHMMSS.ss+DDMMSS.s> N=56+1014+65+1440. Text: <[AGK2012] Cep OB3b East> N=1, <[AGK2012] Cep OB3b West> N=1.
=E=	Catalogue in electronic form as <J/ApJ/750/125/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AGK2018]
[AGK2018]	(Adami+Giles+Koulouridis+, 2018)
Write:	<<[AGK2018] XLSSC 110 NN>> <<[AGK2018] XLSSC 110 AN>>
N:	10+7
Object:	G (SIMBAD class: Galaxy)
Note:	N=10+7 galaxies in the field of the XLSSC 110 galaxy cluster.
in source:	XLSSC 110
Ref:	=2018A&A...620A...5A
by	ADAMI C. , GILES P., KOULOURIDIS E., PACAUD F., CARETTA C.A., PIERRE M., ECKERT D., RAMOS-CEJA M.E., GASTALDELLO F., FOTOPOULOU S., GUGLIELMO V., LIDMAN C., SADIBEKOVA T., IOVINO A., MAUGHAN B., CHIAPPETTI L., ALIS S., ALTIERI B., BALDRY I., BOTTINI D., BIRKINSHAW M., BREMER M., BROWN M., CUCCIATI O., DRIVER S., ELMER E., ETTORI S., EVRARD A.E., FACCIOLI L., GRANETT B., GROOTES M., GUZZO L., HOPKINS A., HORELLOU C., LEFEVRE J.P., LISKE J., MALEK K., MARULLI F., MAUROGORDATO S., OWERS M., PALTANI S., POGGIANTI B., POLLETTA M., PLIONIS M., POLLO A., POMPEI E., PONMAN T., RAPETTI D., RICCI M., ROBOTHAM A., TUFFS R., TASCA L., VALTCHANOV I., VERGANI D., WAGNER G., WILLIS J., (The XXL Consortium)
	Astron. Astrophys., 620A, 5-5 (2018)
	The XXL Survey. XX. The 365 cluster catalogue.
o	Appendix B. CFHT-W CL J021757.8-045142 not in SIMBAD.
o	Tables 5+G.1: <XLSSC NNN> N=302+39 among (Nos 001-642). Table 9: <XLSSsC WNN> (Nos N01-N21, S01-S14). Fig. 16, Table 10: <[AGK2018] XLSSC 110 NN> (Nos 1-10), <[AGK2018] XLSSC 110 AN> (Nos A3-A4, B2-B5, C2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AGK3
AGK3	(Astr. Gesellschaft Katalog, 3rd version)
====>	Equivalent to: AG
Details on Acronym: AGK3R
AGK3R	(Astr. Gesellschaft Katalog, 3rd version, Reference stars)
====>	Equivalent to: AGKR
Details on Acronym: AGK3U
AGK3U	(AGK3 Updated)
====>	Equivalent to: AG
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AGK90]
[AGK90]	(Anderson+Gorham+Kulkarni+, 1990)
Write:	<<[AGK90] 2127+11A>>
N:	8
Object:	ms Psr (SIMBAD class: Pulsar)
Stat:	is completely incorporated in Simbad
Note:	Millisecond pulsars in M 15. (Nos D-H) are added in 1992, Anderson S.B. Ph.D. Thesis, Caltech, and all the pulsars are in 1993ApJS...88..529T.
in source:	NGC 7078 = M 15
Ref:	=1990Natur.346...42A
by	ANDERSON S.B. , GORHAM P.W., KULKARNI S.R., PRINCE T.A., WOLSZCZAN A.
	Nature, 346, 42-None (1990)
	Discovery of two radio pulsars in the globular cluster M 15.
o	Table 1: <[AGK90] 2127+11A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AGKR
AGKR	(Astr. Gesellschaft Katalog, Reference *)= AGK3R
Write:	<<AGKR NNNNN>>
N:	21499
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1978IAUCo..48..505C
by	CORBIN T.E.
	IAU Coll. 48 held in Vienna Austria, September 11-14,1978 "Modern Astrometry",pp, 48, 505-514 (1978)
	The Proper Motions of the AGK3 R and SRS stars.
o	Catalog: <AGKR NNNNN> (Nos 1-21499).
=E=	Catalogue in electronic form as I/161
Details on Acronym: AGL
AGL	(AGILE)
Write:	<<AGL JHHMM+DDMM>>
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	Italian gamma-ray satellite AGILE (Astro-rivelatore Gamma a Immagini LEggero) observations. First references with AGL objects.
Ref:	=2008ATel.1585....1C
by	CHEN A. , CARAVEO P., GIULIANI A., MEREGHETTI S., PELLIZZONI A., VERCELLONE S., PEROTTI F., FORNARI F., FIORINI M., ZAMBRA A., TAVANI M., PUCELLA G., D'AMMANDO F., VITTORINI V., COSTA E., FEROCI M., DONNARUMMA I., PACCIANI L., DEL MONTE E., LAZZAROTTO F., SOFFITTA P., EVANGELISTA Y., LAPSHOV I., RAPISARDA M., ARGAN A., TROIS A., DE PARIS G., BULGARELLI A., GIANOTTI F., TRIFOGLIO M., DI COCCO G., LABANTI C., FUSCHINO F., MARISALDI M., GALLI M., BARBIELLINI G., LONGO F., VALLAZZA E., PICOZZA P., MORSELLI A., PREST M., LIPARI P., ZANELLO D., CATTANEO P., PITTORI C., VERRECCHIA F., PREGER B., SANTOLAMAZZA P., GIOMMI P.
	ATel, 1585, 1 (2008)
	AGILE detection of the flaring γ-ray source AGL2021+4029: a possible rebrightening of a strong source in the Cygnus region.
o	Text: <AGL JHHMM+DDMM> N=1.
Ref:	=2008ApJ...688L..33H
by	HALPERN J.P. , CAMILO F., GIULIANI A., GOTTHELF E.V., McLAUGHLIN M.A., MUKHERJEE R., PELLIZZONI A., RANSOM S.M., ROBERTS M.S.E., TAVANI M.
	Astrophys. J., 688L, 33-36 (2008)
	Discovery of high-energy γ-ray pulsations from PSR J2021+3651 with AGILE.
o	Text: <AGL JHHMM+DDMM> N=1.
Ref:	=2009A&A...494L..33R
by	ROMERO G.E. , VILA G.S.
	Astron. Astrophys., 494L, 33-36 (2009)
	On the nature of the AGILE Galactic transient sources.
o	In reflist LONGO 2008ATel.1429.1L is a misprint for 2008ATel.1492.1L .
o	Text: <AGL JHHMM+DDMM> N=2.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 1AGL
1AGL	(First AGILE catalog of high confidence gamma-ray sources)
Write:	<<1AGL JHHMM+DDMM>>
N:	47
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	First catalog of high confidence gamma-ray sources detected by the AGILE satellite. This catalog is based on Gamma-Ray Imaging Detector (GRID) data for energies greater than 100MeV.
Ref:	=2009A&A...506.1563P
by	PITTORI C. , VERRECCHIA F., CHEN A.W., BULGARELLI A., PELLIZZONI A., GIULIANI A., VERCELLONE S., LONGO F., TAVANI M., GIOMMI P., BARBIELLINI G., TRIFOGLIO M., GIANOTTI F., ARGAN A., ANTONELLI A., BOFFELLI F., CARAVEO P., CATTANEO P.W., COCCO V., COLAFRANCESCO S., CONTESSI T., COSTA E., CUTINI S., D'AMMANDO F., DEL MONTE E., DE PARIS G., DI COCCO G., DI PERSIO G., DONNARUMMA I., EVANGELISTA Y., FANARI G., FEROCI M., FERRARI A., FIORINI M., FORNARI F., FUSCHINO F., FROYSLAND T., FRUTTI M., GALLI M., GASPARRINI D., LABANTI C., LAPSHOV I., LAZZAROTTO F., LIELLO F., LIPARI P., MATTAINI E., MARISALDI M., MASTROPIETRO M., MAURI A., MAURI F., MEREGHETTI S., MORELLI E., MORETTI E., MORSELLI A., PACCIANI L., PEROTTI F., PIANO G., PICOZZA P., PILIA M., PONTONI C., PORROVECCHIO G., PREGER B., PREST M., PRIMAVERA R., PUCELLA G., RAPISARDA M., RAPPOLDI A., ROSSI E., RUBINI A., SABATINI S., SANTOLAMAZZA P., SCALISE E., SOFFITTA P., STELLATO S., STRIANI E., TAMBURELLI F., TRACI A., TROIS A., VALLAZZA E., VITTORINI V., ZAMBRA A., ZANELLO D., SALOTTI L.
	Astron. Astrophys., 506, 1563-1574 (2009)
	First AGILE catalog of high-confidence γ-ray sources.
o	Table 3: <1AGL JHHMM+DDMM> N=47.
=E=	Catalogue in electronic form as J/A+A/506/1563
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 2AGL
2AGL	(Second AGILE-GRID catalog)
Write:	<<2AGL JHHMM+DDMM>> <<2AGL JHHMM+DDMM{c\|e}>>
N:	175
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Second catalog of high confidence gamma-ray sources detected by the AGILE satellite. This catalog is based on Gamma-Ray Imaging Detector (GRID) data for energies in the 100MeV-10GeV range. A letter "c" at the end of the format indicates that the source is considered to be potentially confused with Galactic diffuse emission. A letter "e" at the end of the format indicates that the source was included as an extended source in the analysis. See also 1AGL.
Ref:	=2019A&A...627A..13B
by	BULGARELLI A. , FIORETTI V., PARMIGGIANI N., VERRECCHIA F., PITTORI C., LUCARELLI F., TAVANI M., ABOUDAN A., CARDILLO M., GIULIANI A., CATTANEO P.W., CHEN A.W., PIANO G., RAPPOLDI A., BARONCELLI L., ARGAN A., ANTONELLI L.A., DONNARUMMA I., GIANOTTI F., GIOMMI P., GIUSTI M., LONGO F., PELLIZZONI A., PILIA M., TRIFOGLIO M., TROIS A., VERCELLONE S., ZOLI A.
	Astron. Astrophys., 627A, 13-13 (2019)
	Second AGILE catalogue of γ-ray sources.
o	Tables 10-11: <2AGL JHHMM+DDMM> N=161, <2AGL JHHMM+DDMMc> N=10, <2AGL JHHMM+DDMMe> N=4.
=E=	Catalogue in electronic form as <J/A+A/627/A13/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 1AGLR
1AGLR	(1AGL Revised)
Write:	<<1AGLR JHHMM+DDMM>>
N:	35
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Repositioned and new sources from the first AGILE catalogue of γ-ray sources (1AGL): 8 new high galactic latitude sources, 8 new sources on the galactic plane, and 20 sources from the previous catalogue with revised positions. See also the interactive on-line version, available at http://www.asdc.asi.it/agile1rcat/
Ref:	=2013A&A...558A.137V
by	VERRECCHIA F. , PITTORI C., CHEN A.W., BULGARELLI A., TAVANI M., LUCARELLI F., GIOMMI P., VERCELLONE S., PELLIZZONI A., GIULIANI A., LONGO F., BARBIELLINI G., TRIFOGLIO M., GIANOTTI F., ARGAN A., ANTONELLI L.A., CARAVEO P., CARDILLO M., CATTANEO P.W., COCCO V., COLAFRANCESCO S., CONTESSI T., COSTA E., DEL MONTE E., DE PARIS G., DI COCCO G., DI PERSIO G., DONNARUMMA I., EVANGELISTA Y., FANARI G., FEROCI M., FERRARI A., FIORINI M., FORNARI F., FUSCHINO F., FROYSLAND T., FRUTTI M., GALLI M., LABANTI C., LAPSHOV I., LAZZAROTTO F., LIELLO F., LIPARI P., MATTAINI E., MARISALDI M., MASTROPIETRO M., MAURI A., MAURI F., MEREGHETTI S., MORELLI E., MORETTI E., MORSELLI A., PACCIANI L., PEROTTI F., PIANO G., PICOZZA P., PILIA M., PONTONI C., PORROVECCHIO G., PREST M., PRIMAVERA R., PUCELLA G., RAPISARDA M., RAPPOLDI A., ROSSI E., RUBINI A., SABATINI S., SANTOLAMAZZA P., SOFFITTA P., STELLATO S., STRIANI E., TAMBURELLI F., TRACI A., TROIS A., VALLAZZA E., VITTORINI V., ZANELLO D., SALOTTI L., VALENTINI G.
	Astron. Astrophys., 558A, 137-137 (2013)
	An updated list of AGILE bright γ-ray sources and their variability in pointing mode.
o	<1AGLR JHHMM+DDMM> N=35.
=E=	Catalogue in electronic form as J/A+A/558/A137
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AGM
AGM	(Aparicio+Garcia-Pelayo+Moles+)
Write:	<<AGM Sextans A NNNN>> <<AGM DDO 187 NN>> <<AGM GR 8 NNN>>
N:	2279+77+142
Object:	* (SIMBAD class: Star)
Note:	1987A&AS...71..297A: * in Sextans A format 'Sextans A NNNN', (Nos 1-2279) 1988A&AS...74..367A: * in DDO 187 format 'DDO 187 NN', (Nos 1-77) 1988A&AS...74..375A: * in GRDG 8 format 'GR 8 NNN', (Nos 1-142) Identif. charts
in source:	Sextans A = DDO 75
in source:	DDO 187
in source:	GRDG 8
Ref:	=1987A&AS...71..297A
by	APARICIO A. , GARCIA-PELAYO J.M., MOLES M., MELNICK J.
	Astron. Astrophys., Suppl. Ser., 71, 297-338 (1987)
	CCD photometry of resolved dwarf irregular galaxies. I. Sextans A.
o	(Erratum) vol 72, 367
o	<AGM Sextans A NNNN> (Nos 1-2279)
Ref:	=1988A&AS...74..367A
by	APARICIO A. , GARCIA-PELAYO J.M., MOLES M.
	Astron. Astrophys., Suppl. Ser., 74, 367-374 (1988)
	CCD photometry of resolved dwarf irregular galaxies. II. DDO 187.
o	<AGM DDO 187 NN> (Nos 1-77)
Ref:	=1988A&AS...74..375A
by	APARICIO A. , GARCIA-PELAYO J.M., MOLES M.
	Astron. Astrophys., Suppl. Ser., 74, 375-384 (1988)
	CCD photometry of resolved dwarf irregular galaxies. III. GR 8.
o	<AGM GR 8 NNN> (Nos 1-142)
=E=	Catalogue in electronic form as <J/A+AS/71/297/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AGM87]
[AGM87]	(Aparicio+Garcia-Pelayo+Moles+, 1987)
*****	Avoid the usage of [AGM87], prefer AGM
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AGM88]
[AGM88]	(Aparicio+Garcia-Pelayo+Moles, 1988)
*****	Avoid the usage of [AGM88], prefer AGM
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AGN
AGN	(Atlas of Gal. Nebula)
**	catalog: use GN
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [AGO2007]
[AGO2007]	(Arnaboldi+Gerhard+Okamura+, 2007)= (IPN)
Write:	<<[AGO2007] NNN>>
N:	14+26
Object:	Poss. PN (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
Stat:	is completely incorporated in Simbad
Note:	Subaru FOCAS telescope observations with FOCAS of the Coma Cluster. Detection of 40 PNs in 2 chips (Nos 1, 2).
in source:	Coma Cluster = ACO 1656
Ref:	=2007PASJ...59..419A
by	ARNABOLDI M. , GERHARD O., OKAMURA S., KASHIKAWA N., YASUDA N., FREEMAN K.C.
	PASJ, 59, 419-425 (2007)
	Multi-slit imaging spectroscopy technique: catalog of intracluster planetary nebulae in the Coma cluster.
o	Table 2: <[AGO2007] NNN> (Nos 101-114, 201-226).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AGP
AGP	(Andromeda Galaxy, Amplified Pixel Experiment)
*****	Avoid the usage of AGP, prefer AGAPE
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AGP
AGP	(Ali+Gajdosik+Pfleiderer)
Write:	<<AGP N>>
N:	2
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	'AGP' is an abbreviation of the discoverers' surnames AGP 1 = PN G044.7+00.2, AGP 2 = PN G044.9-00.0
Ref:	=1997MNRAS.289..589A
by	ALI A. , PFLEIDERER J.
	Mon. Not. R. Astron. Soc., 289, 589-591 (1997)
	Two new evolved neighbouring planetary nebulae in Aquila.
o	Table 1: <AGP N> (Nos 1-2)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AGP2018]
[AGP2018]	(Alves+Girart+Padovani+, 2018) (Not yet in Simbad)
Write:	<<[AGP2018] B59 VLA 5a>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Karl G. Jansky VLA 34.5GHz observations of N=2 components of the binary system [DRA2013] B59 VLA 5.
in source:	[DRA2013] B59 VLA 5
Ref:	=2018A&A...616A..56A
by	ALVES F.O. , GIRART J.M., PADOVANI M., GALLI D., FRANCO G.A.P., CASELLI P., VLEMMINGS W.H.T., ZHANG Q., WIESEMEYER H.
	Astron. Astrophys., 616A, 56-56 (2018)
	Magnetic field in a young circumbinary disk.
o	Paragr. 2.2: <[AGP2018] B59 VLA 5a> (Nos 5a-5b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AGP75]
[AGP75]	(Austin+Godwin+Peach, 1975) (Not yet in Simbad)
Write:	<<[AGP75] NNN>>
N:	117
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	See also [AP74], BGP, GP, [GP82]
in source:	ACO 1930
Ref:	=1975MNRAS.171..135A
by	AUSTIN T.B. , GODWIN J.G., PEACH J.V.
	Mon. Not. R. Astron. Soc., 171, 135-142 (1975)
	Studies of rich clusters of galaxies. III. Photometry of the cluster A 1930 and the m-z relation.*
o	Table I: <[AGP75] NNN> (Nos 1-117)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AGPRS
AGPRS	(AGAPE-EROS)
Write:	<<AGPRS JHHMMSS.ss+DDMMSS.s>>
N:	631
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2000A&AS..145...11M
by	MELCHIOR A.-L. , HUGHES S.M.G., GUIBERT J.
	Astron. Astrophys., Suppl. Ser., 145, 11-49 (2000)
	AGAPEROS: Searching for variable stars in the LMC Bar with the Pixel Method. I. Detection, astrometry and cross-identification.
o	Format in the electronic catalogue and in SIMBAD is AGPRS JHHMMSS.ss+DDMMSS.s (2000 coordinates).
o	Table 2: <AGPRS JHHMMSS.ss+DDMMSS.s> N=631.
=E=	Catalogue in electronic form as J/A+AS/145/11
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AGPV
AGPV	(Andromeda Galaxy, Amplified Pixel Experiment, V*)
*****	Avoid the usage of AGPV, prefer AGAPE
Origin	of the Acronym: L (2005A&A...442..879P)
Details on Acronym: [AGS2011]
[AGS2011]	(Ahumada+Giorgi+Solivella+, 2011)
Write:	<<[AGS2011] NNNN>> <<[AGS2011] NNNNN>>
N:	3329+5
Object:	* (SIMBAD class: Star)
Note:	CTIO 1m telescope photometry and CASLEO Observatory 2.1m telescope spectroscopy of the open cluster NGC 4852.
in source:	NGC 4852
Ref:	=2011MNRAS.415.1355A
by	AHUMADA J.A. , GIORGI E.E., SOLIVELLA G., VAZQUEZ R.A.
	Mon. Not. R. Astron. Soc., 415, 1355-1365 (2011)
	Early-type stars in the open cluster NGC 4852.
o	Table 3: <[AGS2011] NNNN> (Nos 1-3329), <[AGS2011] NNNNN> (Nos 10001-10005).
=E=	Catalogue in electronic form as J/MNRAS/415/1355
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AGS2012]
[AGS2012]	(Anderson+Gaensler+Slane+, 2012)
Write:	<<[AGS2012] A>>
N:	4 (SIMBAD class: Radio = Radio Source)
Note:	ATCA 5 and 9 GHz observations of the field of PSR J1622-4950.
Ref:	=2012ApJ...751...53A
by	ANDERSON G.E. , GAENSLER B.M., SLANE P.O., REA N., KAPLAN D.L., POSSELT B., LEVIN L., JOHNSTON S., MURRAY S.S., BROGAN C.L., BAILES M., BATES S., BENJAMIN R.A., BHAT N.D.R., BURGAY M., BURKE-SPOLAOR S., CHAKRABARTY D., D'AMICO N., DRAKE J.J., ESPOSITO P., GRINDLAY J.E., HONG J., ISRAEL G.L., KEITH M.J., KRAMER M., LAZIO T.J.W., LEE J.C., MAUERHAN J.C., MILIA S., POSSENTI A., STAPPERS B., STEEGHS D.T.H.
	Astrophys. J., 751, 53 (2012)
	Multi-wavelength observations of the radio magnetar PSR J1622-4950 and discovery of its possibly associated supernova remnant.
o	Figure 2: <[AGS2012] A> N=4 (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Aguero
Aguero	(Aguero)
Write:	<<Aguero NN>>
N:	48 among 84
Object:	G (SIMBAD class: Galaxy)
Ref:	=1971PASP...83..310A
by	AGUERO E.L.
	Publ. Astron. Soc. Pac., 83, 310-312 (1971)
	A list of interesting southern galaxies.
o	Table I: <Aguero NN> N=48 among (Nos 1-84)
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: AH
AH	(A. Hoag)
Write:	<<AH NN>>
N:	28
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Ref:	=1986IAUS..119...47H
by	HOAG A.
	IAU Symp., 119, held in Bangladore, India, Dec 2-6, 1985. Ed. G. Swarup and V.K. Kapahi. " Quasars", 1986, 119, 47-48 (1986)
	QSO search by slitless spectroscopy.
o	<AH NN> (Nos 1-28)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: AH
AH	(Aveni+Hunter)= (Aveni-Hunter)
Write:	<<Cl AH N>>
N:	1
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Ref:	=1969AJ.....74.1021A
by	AVENI A.F. , HUNTER J.H.
	Astron. J., 74, 1021-None (1969)
	Observational studies relating to star formation. II.
o	<Cl AH 1> = <NAME AVENI-HUNTER 1>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AH2000]
[AH2000]	(Aalto+Huttemeister, 2000)
Write:	<<[AH2000] Peak a>>
N:	5
Object:	Em. peak (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Fig. 8a: map of 12CO peaks in molecular emission in NGC 4194.
in source:	NGC 4194
Ref:	=2000A&A...362...42A
by	AALTO S. , HUETTEMEISTER S.
	Astron. Astrophys., 362, 42-52 (2000)
	Complex molecular gas structure in the Medusa merger.
o	Table 3: <[AH2000] Peak a> (Nos a-e).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AH2003]
[AH2003]	(Alves+Homeier, 2003)
Write:	<<[AH2003] N>>
N:	4
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	SofI NIR observations on the ESO NTT telescope. N=4 massive stellar clusters embedded in W 49A.
in source:	W 49:W 49A = W 49A
Ref:	=2003ApJ...589L..45A
by	ALVES J. , HOMEIER N.
	Astrophys. J., 589, 45-49 (2003)
	Uncovering the beast: discovery of embedded massive stellar clusters in W49A.
o	Fig.1: radio sources = [DJW84] W49 AN
o	Fig.3, Table 1: <[AH2003] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AH2005]
[AH2005]	(Alvarez+Hoare, 2005)
Write:	<<[AH2005] Mon R2 A>> <<[AH2005] S255 A>> <<[AH2005] GL 961 A>> <<[AH2005] GL 989 A>> <<[AH2005] Mon R2W N>> <<[AH2005] S255 N>> <<[AH2005] GL 961 N>> <<[AH2005] GL 989 NN>>
N:	7+28
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Note:	Taurus Tunable Filter observations at the AAT of shock excited emission lines in outflows from massive YSO. Format ending by a letter: emission line features in each object. Format ending by a number: emission line stars in the field of each object.
in source:	NAME Mon R2 GMC
in source:	SH 2-255
in source:	RAFGL 961
in source:	RAFGL 989
Ref:	=2005A&A...440..569A
by	ALVAREZ C. , HOARE M.G.
	Astron. Astrophys., 440, 569-581 (2005)
	A search for shock-excited optical emission from the outflows of massive young stellar objects.
o	in ref list ALLEN 1972ApL....12..231A instead of ApJ.12.231
o	Table 2: <[AH2005] Mon R2 A> (Nos A-C), <[AH2005] S255 A> (No. A), <[AH2005] GL 961 A> (Nos A-B), <[AH2005] GL 989 A> (No. A). Table 3: <[AH2005] Mon R2W N> (Nos R2N 1 to 3, R2S 1 to 2), <[AH2005] S255 N> (Nos 1-8), <[AH2005] GL 961 N> (Nos 1-2), <[AH2005] GL 989 NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AH80]
[AH80]	(Arp+Hazard, 1980)
Write:	<<[AH80] 1146+111 A>> <<[AH80] 1130+106 A>>
N:	20+6
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Note:	Fig.1: N=20 QSO candidates in the field 1146+111, among which 9 QSO are in T.1 Fig.2 and T.1: N=6 QSO in the field 1130+106
Ref:	=1980ApJ...240..726A
by	ARP H. , HAZARD C.
	Astrophys. J., 240, 726-736 (1980)
	Peculiar configurations of quasars in two adjacent areas of the sky.
o	Table 1, Fig1, Fig2: <[AH80] 1146+111 A> (Nos A-T), <[AH80] 1130+106 A> (Nos A-C, X-Z)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AHA2018]
[AHA2018]	(Aso+Hirano+Aikawa+, 2018)
Write:	<<[AHA2018] Serpens SMM4A>>
N:	2
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	ALMA 1.3mm continuum observations of N=2 protostars in Serpens SMM 4.
in source:	NAME Serpens SMM 4
Ref:	=2018ApJ...863...19A
by	ASO Y. , HIRANO N., AIKAWA Y., MACHIDA M.N., TAKAKUWA S., YEN H.-W., WILLIAMS J.P.
	Astrophys. J., 863, 19-19 (2018)
	The distinct evolutionary nature of two Class 0 protostars in Serpens Main SMM4.
o	Fig. 1: <[AHA2018] Serpens SMM4A> (Nos SMM4A-SMM4B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AHB2012]
[AHB2012]	(Antoja+Helmi+Bienayme+, 2012)
Write:	<<[AHB2012] NN>>
N:	19
Object:	Moving Group (SIMBAD class: MouvGroup = Moving Group)
Note:	N=19 moving groups in RAVE data.
Ref:	=2012MNRAS.426L...1A
by	ANTOJA T. , HELMI A., BIENAYME O., BLAND-HAWTHORN J., FAMAEY B., FREEMAN K., GIBSON B.K., GILMORE G., GREBEL E.K., MINCHEV I., MUNARI U., NAVARRO J., PARKER Q., REID W., SEABROKE G.M., SIEBERT A., SIVIERO A., STEINMETZ M., WILLIAMS M., WYSE R., ZWITTER T.
	Mon. Not. R. Astron. Soc., 426L, 1-5 (2012)
	Kinematic groups beyond the solar neighbourhood with RAVE.
o	Some kinematic structures Table 2 are not in Simbad.
o	Table 2: <[AHB2012] NN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AHB74]
[AHB74]	(Akyol+Hidajat+Balazs+, 1974) (Not yet in Simbad)
Write:	<<[AHB74] Red NN>> <<[AHB74] M NNN>> <<[AHB74] C NN>> <<[AHB74] V NN>>
N:	492
Object:	* (SIMBAD class: Star)
Note:	Appendix I to IV: Spectral survey of IR stars, N=37 reddened early type stars, format 'Red NN', (format 'App I NN' for the authors), N=369 M type stars, format 'M NNN', (format 'App II NNN' for the authors), N=54 Carbon stars, format 'C NN', (format 'App III NN' for the authors), N=32 Variable stars, format 'V NN'. (format 'App IV NN' for the authors),
Ref:	=1974A&AS...18..427A
by	AKYOL M.U. , HIDAJAT B., BALAZS L.G., VOELCKER K.
	Astron. Astrophys., Suppl. Ser., 18, 427-445 (1974)
	A photographic search for red stars in Aquila-Cygnus.
o	= 1974CoBos.55 Authors use formats 'App I NNN' to 'App IV NNN' whe re App stands for Appendix, instead of those used in SIMBAD.
o	Appendix I: <[AHB74] Red NN> (Nos 1-37). Appendix II: <[AHB74] M NNN> (Nos 1-369). Appendix III: <[AHB74] C NN> (Nos 1-54). Appendix IV: <[AHB74] V NN> (Nos 1-32).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AHE2022]
[AHE2022]	(Archer+Hunter+Elmegreen+, 2022)
Write:	<<[AHE2022] NN>>
N:	26
Object:	Star Forming Region (SIMBAD class: StarFormingReg = Star Forming Region)
Stat:	is completely incorporated in Simbad
Note:	N=26 star forming regions in the WLM galaxy.
in source:	DDO 221 = NAME WLM Galaxy
Ref:	=2022AJ....163..141A
by	ARCHER H.N. , HUNTER D.A., ELMEGREEN B.G., CIGAN P., JANSEN R.A., WINDHORST R.A., HUNT L.K., RUBIO M.
	Astron. J., 163, 141-141 (2022)
	The environments of CO cores and star formation in the dwarf irregular galaxy WLM.
o	Table 1: <[AHE2022] NN> (Nos 1-26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AHG2004]
[AHG2004]	(Alvarez+Hoare+Glindemann+, 2004)
Write:	<<[AHG2004] GL 961-Fan>> <<[AHG2004] NGC 7538 IRS A>> <<[AHG2004] NGC 7538 Star a>> <<[AHG2004] GL 5180 IRS 1 A>>
N:	1+3+6+4
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Near-IR speckle images of YSOs, from IRCAM3 at UKIRT. Near AFGL 961 lies an optical fan-shaped nebula, designated as 'GL 961-Fan' by the authors. In the field of NGC 7538 authors observed 3 extended features which are part of the NIR nebula '[TGJ91] NGC 7538 IRS 1 IRN', and 6 stars a to f. In the image of '[TGJ91] AFGL 5180 NIRS 1', 4 new IR sources are found, sources A and B are two components of a binary.
Ref:	=2004A&A...427..505A
by	ALVAREZ C. , HOARE M., GLINDEMANN A., RICHICHI A.
	Astron. Astrophys., 427, 505-518 (2004)
	Near-IR speckle imaging of massive young stellar objects.
o	Fig.10, Table 1: <[AHG2004] GL 961-Fan> N=1. Fig.14: <[AHG2004] NGC 7538 IRS A> (Nos A-C), <[AHG2004] NGC 7538 Star a> (Nos a-f). Fig.15: <[AHG2004] GL 5180 IRS 1 A> (Nos A-D). Fig.10, Table 1: <[LHR84] GL 961 Wa> (Nos Wa, Wb) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AHH
AHH	(Allen+Hyland+Hillier)
N:	1
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1990MNRAS.244..706A
by	ALLEN D.A. , HYLAND A.R., HILLIER D.J.
	Mon. Not. R. Astron. Soc., 244, 706-713 (1990)
	The source of luminosity at the Galactic Centre.
o	<NAME AHH STAR> N=1.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AHH2015]
[AHH2015]	(Adams+Herter+Hora+, 2015)
Write:	<<[AHH2015] {C\|W\|S\|P}{L} N>>
N:	7+3+3+1
Object:	(Mid IR) (SIMBAD class: FarIR = Far-IR source (λ >= 30 µm))
Stat:	is completely incorporated in Simbad
Note:	SOFIA FORCAST mid-IR observations of N=20 warm dust sources in S106. Use of Spitzer IRAC, IRTF MIRLIN and Herschel PACS data.
in source:	NAME S106 FIR
Ref:	=2015ApJ...814...54A
by	ADAMS J.D. , HERTER T.L., HORA J.L., SCHNEIDER N., LAU R.M., STAGUHN J.G., SIMON R., SMITH N., GEHRZ R.D., ALLEN L.E., BONTEMPS S., CAREY S.J., FAZIO G.G., GUTERMUTH R.A., GUZMAN FERNANDEZ A., HANKINS M., HILL T., KETO E., KOENIG X.P., KRAEMER K.E., MEGEATH S.T., MIZUNO D.R., MOTTE F., MYERS P.C., SMITH H.A.
	Astrophys. J., 814, 54 (2015)
	SOFIA/FORCAST observations of warm dust in S106: a fragmented environment.
o	Table 2: <[AHH2015] CL N> (Nos CL 1-Cl 7), <[AHH2015] WL N> (Nos WL 1-WL 3), <[AHH2015] SL N> (Nos SL 1-SL 3), <[AHH2015] PL N> (No PL 1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AHK74]
[AHK74]	(Arp+Heidmann+Khachikyan, 1974)
Write:	<<[AHK74] aN>>
N:	6
Object:	G (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spectroscopic observations at the 6m SAO telescope of N=6 condensations in the fields of Mrk 261, 262. The object e has at least two components.
Ref:	=1974Afz....10....7A
by	ARP H.C. , HEIDMANN J., KHACHIKYAN E.E.
	Astrofizika, 10, 7-12 (1974)
	Remarkable pair of double galaxies.
o	Fig.4: <[AHK74] a> (Nos a-f).
Ref:	=2005Ap.....48..422K
by	KHACHIKIAN E.Y. , SARGSYAN L.A.
	Astrophysics, 48, 422-432 (2005)
	Spectrophotometric study of the region of the sky around the galaxies Markarian 261 and 262.
o	Fig.2, Table 2: <[AHK74] aN> (Nos e1-e2) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AHL2004]
[AHL2004]	(Araya+Hofner+Linz+, 2004)= (IRDC)
Write:	<<[AHL2004] JHHMM+DD>>
N:	3
Object:	Cloud (SIMBAD class: Cloud)
Note:	Arcibo observations of infrared dark clouds from the MSX Galactic Plane Survey.
Ref:	=2004ApJS..154..579A
by	ARAYA E. , HOFNER P., LINZ H., SEWILO M., WATSON C., CHURCHWELL E., OLMI L., KURTZ S.
	Astrophys. J., Suppl. Ser., 154, 579-584 (2004)
	A search for H_{2}CO 6 centimeter emission toward young massive stellar objects.
o	Table 1: <[AHL2004] JHHMM+DD> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AHP2000]
[AHP2000]	(Andersen+Hjorth+Pedersen+, 2000) (Not yet in Simbad)
Write:	<<[AHP2000] A>>
N:	4
Object:	* (SIMBAD class: Star)
Note:	N=4 reference stars in the field of GRB 000131.
Ref:	=2000A&A...364L..54A
by	ANDERSEN M.I. , HJORTH J., PEDERSEN H., JENSEN B.L., HUNT L.K., GOROSABEL J., MOLLER P., FYNBO J., KIPPEN R.M., THOMSEN B., OLSEN L.F., CHRISTENSEN L., VESTERGAARD M., MASETTI N., PALAZZI E., HURLEY K., CLINE T., KAPER L., JAUNSEN A.O.
	Astron. Astrophys., 364, 54-61 (2000)
	VLT identification of the optical afterglow of the γ-ray burst GRB 000131 at z=4.50.
o	Fig.3, Table 3: <[AHP2000] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AHP2016]
[AHP2016]	(Alexander+Hanes+Povich+, 2016)
Write:	<<[AHP2016] OBc NN>>
N:	94
Object:	Poss. OB* (SIMBAD class: Star)
Note:	AAT AAOmega 2dF spectroscopic observations of N=94 OB star candidates in the Carina Nebula.
in source:	NGC 3372 = NAME Carina Nebula
Ref:	=2016AJ....152..190A
by	ALEXANDER M.J. , HANES R.J., POVICH M.S., McSWAIN M.V.
	Astron. J., 152, 190-190 (2016)
	A catalog of new spectroscopically confirmed massive OB stars in Carina.
o	Fig. 2, Tables 3-4: <[AHP2016] OBc NN> (Nos 1-94).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AHS99]
[AHS99]	(Aalto+Huttemeister+Scoville+, 1999)
Write:	<<[AHS99] {M\|C\|S\|B\|D}N>>
N:	11
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Note:	CO map of W 51: N=2 arms (Nos M1-M2), N=1 peculiar feature (No. C), N=5 molecular spurs (Nos S1-S5), N=2 faint chain of MCld (Nos B1-B2), N=1 chain of interarm clouds (No. D).
in source:	M 51 = NGC 5194
Ref:	=1999ApJ...522..165A
by	AALTO S. , HUETTEMEISTER S., SCOVILLE N.Z., THADDEUS P.
	Astrophys. J., 522, 165-182 (1999)
	A new high-resolution CO map of the inner 2'.5 of M51. I. Streaming motions and spiral structure.
o	Figs 1,6: Nos among A1 and A10 and Nos IC1 to IC3 = [RK90] ANN and [RK90] I1 to I3.
o	Fig.1: <[AHS99] AN> (Nos M1-M2, C, S1-S5, B1-B2, D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AIC2005]
[AIC2005]	(Agueros+Ivezic+Covey+, 2005)= (GALEX)
Write:	<<[AIC2005] GALEX JHHMMSS.ss+DDMMSS.ss>>
N:	21
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Note:	Properties of SDSS sources detected by GALEX.
Ref:	=2005AJ....130.1022A
by	AGUEROS M.A. , IVEZIC Z., COVEY K.R., OBRIC M., HAO L., WALKOWICZ L.M., WEST A.A., VANDEN BERK D.E., LUPTON R.H., KNAPP G.R., GUNN J.E., RICHARDS G.T., BOCHANSKI J.Jr, BROOKS A., CLAIRE M., HAGGARD D., KAIB N., KIMBALL A., GOGARTEN S.M., SETH A., SOLONTOI M.
	Astron. J., 130, 1022-1036 (2005)
	The ultraviolet, optical, and infrared properties of Sloan Digital Sky Survey sources detected by GALEX.
o	Table 2: <[AIC2005] GALEX JHHMMSS.ss+DDMMSS.ss> N=21.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AIP2008]
[AIP2008]	(Adami+Ilbert+Pello+, 2008)
Write:	<<[AIP2008] GN>>
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	CFHT CFH12K observations of the Coma Cluster. See also [ABD2005].
in source:	Coma Cluster = ACO 1656
Ref:	=2008A&A...491..681A
by	ADAMI C. , ILBERT O., PELLO R., CUILLANDRE J.C., DURRET F., MAZURE A., PICAT J.P., ULMER M.P.
	Astron. Astrophys., 491, 681-692 (2008)
	Photometric redshifts as a tool for studying the Coma cluster galaxy populations.
o	Table 2: <[AIP2008] GN> (Nos G1-G5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AIS2009]
[AIS2009]	(Arbutina+Ilic+Stavrek+, 2009)
Write:	<<[AIS2009] NNA>>
N:	21
Object:	Poss. HII (SIMBAD class: HIIReg = HII Region)
Note:	Rozhen observatory 2m RCC telescope observation of Holmberg IX.
in source:	Holmberg IX
Ref:	=2009SerAJ.179...87A
by	ARBUTINA B. , ILIC D., STAVREV K., UROSEVIC D., VUKOTIC B., ONIC D.
	SerAJ, 179, 87-94 (2009)
	Optical observations of M81 galaxy group in narrow band [SII] and Hα filters: Holmberg IX.
o	Fig. 4, Table 5: <[AIS2009] NNA> (Nos 1-5, 6A-6B, 7A-7B, 8-21).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AIS99]
[AIS99]	(Aschenbach+Iyudin+Schonfelder, 1999)
Write:	<<[AIS99] JHHMMSS+DDMMSS>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	RASS survey in the area of RX J0852.0-4622: N=2 point source candidates.
Ref:	=1999A&A...350..997A
by	ASCHENBACH B. , IYUDIN A.F., SCHOENFELDER V.
	Astron. Astrophys., 350, 997-1006 (1999)
	Constraints of age, distance and progenitor of the supernova remnant RX J0852.0-4622/GRO J0852-4642.
o	text: <[AIS99] JHHMMSS+DDMMSS> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Aitken
Aitken	(Aitken)
*****	Avoid the usage of Aitken, prefer ADS
Details on Acronym: [AJB2003]
[AJB2003]	(Argo+Jackson+Browne+, 2003)
Write:	<<[AJB2003] B0445+123 A>> <<[AJB2003] B0445+123 A'>>
N:	2+2
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Stat:	is completely incorporated in Simbad
Note:	Images of the gravitational lens system CLASS B0445+123. A' and B' are weaker components than A and B.
Ref:	=2003MNRAS.338..957A
by	ARGO M.K. , JACKSON N.J., BROWNE I.W.A., YORK T., McKEAN J.P., BIGGS A.D., BLANDFORD R.D., DE BRUYN A.G., CHAE K.-H., FASSNACHT C.D., KOOPMANS L.V.E., MYERS S.T., NORBURY M., PEARSON T.J., PHILLIPS P.M., READHEAD A.C.S., RUSIN D., WILKINSON P.N.
	Mon. Not. R. Astron. Soc., 338, 957-961 (2003)
	CLASS B0445+123: a new two-image gravitational lens system.
o	Table 2, Fig.2: <[AJB2003] B0445+123 A> (Nos A-B), <[AJB2003] B0445+123 A'> (Nos A'-B').
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AJB2011]
[AJB2011]	(Aversa+Johnson+Brogan+, 2011)
Write:	<<[AJB2011] Arp NNNa>> <<[AJB2011] Arp NNNw>> <<[AJB2011] Mrk NNw>> <<[AJB2011] NGC NNNN>> <<[AJB2011] NGC NNNNa>> <<[AJB2011] NGC NNNNw>> <<[AJB2011] NGC NNNNaw>> <<[AJB2011] NGC 1313snr>>
N:	15+12
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA and ATCA observations of star-forming galaxies.
Ref:	=2011AJ....141..125A
by	AVERSA A.G. , JOHNSON K.E., BROGAN C.L., GOSS W.M., PISANO D.J.
	Astron. J., 141, 125 (2011)
	Very large array and ATCA search for natal star clusters in nearby star-forming galaxies.
o	Tables 3-4: <[AJB2011] Arp NNNa>, <[AJB2011] Arp NNNw>, <[AJB2011] Mrk NNw>, <[AJB2011] NGC NNNN>, <[AJB2011] NGC NNNNw>, <[AJB2011] NGC NNNNa>, <[AJB2011] NGC NNNNaw>, <[AJB2011] NGC 1313snr>, N=15+12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AJG
AJG	(A.J. Green)
Write:	<<AJG NNN>>
N:	117
Object:	SNR (SIMBAD class: SNRemnant = SuperNova Remnant)
Stat:	is completely incorporated in Simbad
Ref:	=1974A&AS...18..267G
by	GREEN A.J.
	Astron. Astrophys., Suppl. Ser., 18, 267-307 (1974)
	The structure of the Milky Way. I. A radio continuum survey of the galactic plane at 408 MHz.
o	Table 2: <AJG NNN> (Nos 1-117).
Origin	of the Acronym: L (1980A&AS...42..227K)
Details on Acronym: [AJG2012]
[AJG2012]	(Adami+Jouvel+Guennou+, 2012)
Write:	<<[AJG2012] DDD.ddddd+DD.ddddd>>
N:	32+43+38
Object:	G (SIMBAD class: Galaxy)
Note:	NTT/EFOSC2 and TNG/Dolores spectroscopic observations of galaxies in the fields of N=3 galaxy groups.
in source:	RX J1119.0+2126
in source:	1RXS J235814.0+150524
in source:	WBL 604
Ref:	=2012A&A...540A.105A
by	ADAMI C. , JOUVEL S., GUENNOU L., LE BRUN V., DURRET F., CLEMENT B., CLERC N., COMERON S., ILBERT O., LIN Y., RUSSEIL D., SEEMANN U.
	Astron. Astrophys., 540A, 105-105 (2012)
	Comparison of the properties of two fossil groups of galaxies with the normal group NGC 6034 based on multiband imaging and optical spectroscopy.
o	Table A.1: <[AJG2012] DDD.ddddd+DD.ddddd> N=32, Table A.3: <[AJG2012] DDD.ddddd+DD.ddddd> N=43, Table A.4: <[AJG2012] DDD.ddddd+DD.ddddd> N=38.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AJM88]
[AJM88]	(Ables+Jacka+McConnell+, 1988)= (MSP)
Write:	<<[AJM88] 0021-72A>>
N:	24
Object:	ms Psr (SIMBAD class: Pulsar)
Stat:	is completely incorporated in Simbad
Note:	Millisecond pulsars in 47 Tuc.
in source:	NGC 104 = 47 Tuc
Ref:	=1988IAUC.4602....0A
by	ABLES J.G. , JACKA C.E., McCONNELL D., HAMILTON P.A., McCULLOCH P.M., HALL P.J.
	IAU Circ., -1-None (1988)
	PSR 0021-72A and 0021-72B.
o	<[AJM88] 0021-72A> (Nos A-B) = <PSR 0021-72A> (Nos A-B).
Ref:	=1991Natur.352..219M
by	MANCHESTER R.N. , LYNE A.G., ROBINSON C., D'AMICO N., BAILES M., LIM J.
	Nature, 352, 219-None (1991)
	Discovery of ten millisecond pulsars in the globular cluster 47 Tucanae.
o	<[AJM88] 0021-72A> (Nos C-M) = <PSR 0021-72A> (Nos C-M) added.
Ref:	=1995MNRAS.274..547R
by	ROBINSON C. , LYNE A.G., MANCHESTER R.N., BAILES M., D'AMICO N., JOHNSTON S.
	Mon. Not. R. Astron. Soc., 274, 547-554 (1995)
	Millisecond pulsars in the globular cluster 47 Tucanae.
o	<[AJM88] 0021-72A> (No. N) = <PSR B0021-72A> (No. N) added.
Ref:	=2000ApJ...535..975C
by	CAMILO F. , LORIMER D.R., FREIRE P.C., LYNE A.G., MANCHESTER R.N.
	Astrophys. J., 535, 975-990 (2000)
	Observations of 20 millisecond pulsars in 47 Tucanae at 20 centimeters.
o	<[AJM88] 0021-72A> (Nos O-W) = <PSR B0021-72A> (Nos O-W) added.
Ref:	=2006ApJ...646.1104B
by	BOGDANOV S. , GRINDLAY J.E., HEINKE C.O., CAMILO F., FREIRE P.C.C., BECKER W.
	Astrophys. J., 646, 1104-1115 (2006)
	Chandra X-ray observations of 19 millisecond pulsars in the globular cluster 47 Tucanae.
o	Table 1: <[AJM88] 0021-72A> (No. Y> = <PSR 0021-72Y> added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AK2012]
[AK2012]	(Alexander+Kobulnicky, 2012)
Write:	<<[AK2012] NN>>
N:	18
Object:	candidate ultracompact embedded cluster (UCEC) (SIMBAD class: Association = Association of Stars)
Stat:	is completely incorporated in Simbad
Note:	Search for ultracompact embedded star clusters in the Galactic plane. Use of archival Spitzer GLIMPSE and UKIDSS data.
Ref:	=2012ApJ...755L..30A
by	ALEXANDER M.J. , KOBULNICKY H.A.
	Astrophys. J., 755L, 30 (2012)
	Ultracompact embedded clusters in the galactic plane.
o	Table 1: <[AK2012] NN> (Nos 1-18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AK2014]
[AK2014]	(Abramson+Kenney, 2014) (Not yet in Simbad)
Write:	<<[AK2014] {NGC 4522\|NGC 4402} {Cloud} NN>>
N:	13+20
Object:	Cloud (SIMBAD class: Cloud)
Note:	HST ACS BVI observations of N=13+20 clouds in NGC 4522 and NGC 4402.
in source:	NGC 4522
in source:	NGC 4402
Ref:	=2014AJ....147...63A
by	ABRAMSON A. , KENNEY J.D.P.
	Astron. J., 147, 63 (2014)
	Hubble Space Telescope imaging of decoupled dust clouds in the ram pressure stripped Virgo spirals NGC 4402 and NGC 4522.
o	Fig. 3, Table 3: <[AK2014] NGC 4522 Cloud NN> (Nos 1-13). Fig. 4, Table 4: <[AK2014] NGC 4402 Cloud NN> (Nos 1-20).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AK3
AK3	(AMICO KiDS-DR3) (Not yet in Simbad)
Write:	<<AK3 JHHMMSS.ss+DDMMSS>>
N:	7988
Object:	Poss. Cluster of G (SIMBAD class: ClG_Candidate = Cluster of Galaxies Candidate)
Note:	N=7988 galaxy cluster candidates in the Kilo-Degree Survey (KiDS) DR3, using the the AdaptiveMatched Identifier of Clustered Objects (AMICO) algorithm.
Ref:	=2019MNRAS.485..498M
by	MATURI M. , BELLAGAMBA F., RADOVICH M., RONCARELLI M., SERENO M., MOSCARDINI L., BARDELLI S., PUDDU E.
	Mon. Not. R. Astron. Soc., 485, 498-512 (2019)
	AMICO galaxy clusters in KiDS-DR3: sample properties and selection function.
o	<AK3 JHHMMSS.ss+DDMMSS> N=7988.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AKARI-FIS-V1
AKARI-FIS-V1	(AKARI/FIS Bright Source Catalogue, Version 1)
Write:	<<AKARI-FIS-V1 JHHMMSSs+DDMMSS>>
N:	427071
Object:	(IR) (SIMBAD class: MidIR = Mid-IR Source (3 to 30 µm))
Note:	AKARI/FIS (Far-Infrared Surveyor) all-sky observations at 65, 90, 140 and 160µ.m. See also AKARI-FIS-V2.
Ref:	=2010yCat.2298....0Y
by	YAMAMURA I. , MAKIUTI S., IKEDA N., FUKUDA Y., OYABU S., KOGA T., WHITE G.J.
	yCat, 2298, 0 (2010)
	AKARI/FIS All-Sky Survey Point Source Catalogues (ISAS/JAXA, 2010).
o	<AKARI-FIS-V1 JHHMMSSs+DDMMSS> N=427071.
=E=	Catalogue in electronic form as II/298
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AKARI-FIS-V2
AKARI-FIS-V2	(AKARI/FIS Bright Source Catalogue, Version 2)
Write:	<<AKARI-FIS-V2 JHHMMSSs+DDMMSS>>
N:	501444+416612
Object:	(IR) (SIMBAD class: MidIR = Mid-IR Source (3 to 30 µm))
Note:	AKARI/FIS (Far-Infrared Surveyor) all-sky observations at 65, 90, 140 and 160µm. The AKARI/FIS Bright Source Catalogue Version 2.0 consists of two parts: the main catalogue of N=501444 sources with high detection reliability and the supplemental catalogue of N=416612 sources which are confirmed at one of four wavelength bands. See also AKARI-FIS-V1.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AKARI-IRC-V1
AKARI-IRC-V1	(AKARI/IRC Point Source Catalogue, Version 1)
Write:	<<AKARI-IRC-V1 JHHMMSSs+DDMMSS>>
N:	870973
Object:	(IR) (SIMBAD class: MidIR = Mid-IR Source (3 to 30 µm))
Note:	AKARI/IRC (InfraRed Camera) all-sky observations at 9mu.m and 18mu.m.
Ref:	=2010A&A...514A...1I
by	ISHIHARA D. , ONAKA T., KATAZA H., SALAMA A., ALFAGEME C., CASSATELLA A., COX N., GARCIA-LARIO P., STEPHENSON C., COHEN M., FUJISHIRO N., FUJIWARA H., HASEGAWA S., ITA Y., KIM W., MATSUHARA H., MURAKAMI H., MUELLER T.G., NAKAGAWA T., OHYAMA Y., OYABU S., PYO J., SAKON I., SHIBAI H., TAKITA S., TANABE T., UEMIZU K., UENO M., USUI F., WADA T., WATARAI H., YAMAMURA I., YAMAUCHI C.
	Astron. Astrophys., 514A, 1-1 (2010)
	The AKARI/IRC mid-infrared all-sky survey.
o	<AKARI-IRC-V1 JHHMMSSs+DDMMSS> N=870973.
=E=	Catalogue in electronic form as II/297
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AKARI-LMCA
AKARI-LMCA	(AKARI-LMC Point Source Archive) (Not yet in Simbad)
Write:	<<AKARI-LMCA JHHMMSS.ss+DDMMSS.s>>
N:	660286
Object:	(IR) (SIMBAD class: MidIR = Mid-IR Source (3 to 30 µm))
Note:	Near- to mid-infrared point source archive of five photometric bands (3.2, 7, 11, 15 and 24µm) of AKARI IRC observations of the Large Magellanic Cloud (LMC). See also the Point Source Catalog AKARI-LMCC. "Archive" includes all detected sources and thus has more and fainter sources than "Catalog", which may contain potential false detection or sources with larger photometric uncertainties.
in source:	Magellanic Clouds:LMC
Ref:	=2012AJ....144..179K
by	KATO D. , ITA Y., ONAKA T., TANABE T., SHIMONISHI T., SAKON I., KANEDA H., KAWAMURA A., WADA T., USUI F., KOO B.-C., MATSUURA M., TAKAHASHI H.
	Astron. J., 144, 179 (2012)
	AKARI Infrared Camera survey of the Large Magellanic Cloud. I. Point-source catalog.
o	<AKARI-LMCC JHHMMSS.ss+DDMMSS.s> N=660286. <AKARI-LMCA JHHMMSS.ss+DDMMSS.s> N=802285.
=E=	Catalogue in electronic form as <J/AJ/144/179/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AKARI-LMCC
AKARI-LMCC	(AKARI-LMC Point Source Catalogue)
Write:	<<AKARI-LMCC JHHMMSS.ss+DDMMSS.s>>
N:	660286
Object:	(IR) (SIMBAD class: MidIR = Mid-IR Source (3 to 30 µm))
Note:	AKARI IRC observations of the Large Magellanic Cloud (LMC). Near- to mid-infrared point source catalog of five photometric bands (3.2, 7, 11, 15 and 24µm). See also the Point Source Archive AKARI-LMCA.
in source:	Magellanic Clouds:LMC
Ref:	=2012AJ....144..179K
by	KATO D. , ITA Y., ONAKA T., TANABE T., SHIMONISHI T., SAKON I., KANEDA H., KAWAMURA A., WADA T., USUI F., KOO B.-C., MATSUURA M., TAKAHASHI H.
	Astron. J., 144, 179 (2012)
	AKARI Infrared Camera survey of the Large Magellanic Cloud. I. Point-source catalog.
o	<AKARI-LMCC JHHMMSS.ss+DDMMSS.s> N=660286. <AKARI-LMCA JHHMMSS.ss+DDMMSS.s> N=802285.
=E=	Catalogue in electronic form as <J/AJ/144/179/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AKARI-NEPD
AKARI-NEPD	(AKARI-North Ecliptic Pole Deep survey)
*****	Avoid the usage of AKARI-NEPD, prefer [TMG2012]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AKB93]
[AKB93]	(Abraham+Kun+Balazs+, 1993)
Write:	<<[AKB93] NN>>
N:	21
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Note:	Finding charts
Ref:	=1993A&A...268..230A
by	ABRAHAM P. , KUN M., BALAZS L.G., HOLL A., FRONTO A.
	Astron. Astrophys., 268, 230-244 (1993)
	Infrared environment of 6 Cephei.
o	<[AKB93] NN> N=21>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AKC2006]
[AKC2006]	(Allers+Kessler-Silacci+Cieza+, 2006)
Write:	<<[AKC2006] NN>>
N:	19
Object:	* (SIMBAD class: Star)
Note:	Spitzer IRAC and MIPS observations. NIR and optical imaging at the CTIO Blanco 4m telescope. Sample of 19 young stars, brown dwarfs, and sub-brown dwarfs with MIR excess.
Ref:	=2006ApJ...644..364A
by	ALLERS K.N. , KESSLER-SILACCI J.E., CIEZA L.A., JAFFE D.T.
	Astrophys. J., 644, 364-377 (2006)
	Young, low-mass brown dwarfs with mid-infrared excesses.
o	Table 3: <[AKC2006] NN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AKC2009]
[AKC2009]	(Alexander+Kobulnicky+Clemens+, 2009)
Write:	<<[AKC2009] Cluster>> <<[AKC2009] NN>>
N:	1+16
Object:	Cluster of * + * in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Spitzer GLIMPSE and MIPSGAL archival data and 1.8m Perkins telescope spectroscopy of a new red supergiant cluster.
Ref:	=2009AJ....137.4824A
by	ALEXANDER M.J. , KOBULNICKY H.A., CLEMENS D.P., JAMESON K., PINNICK A., PAVEL M.
	Astron. J., 137, 4824-4833 (2009)
	The discovery of a massive cluster of red supergiants with GLIMPSE.
o	Text: <[AKC2009] Cluster>. Table 1: <[AKC2009] NN> (Nos 1-16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AKD2020]
[AKD2020]	(Asa'd+Kovalev+Davies+, 2020)
Write:	<<[AKD2020] OB22669NN>>
N:	6
Object:	Red Supergiant (SIMBAD class: RedSG = Red Supergiant)
Note:	VLT X-Shooter observations of N=6 red supergiants stars in the young massive cluster VdBH 222.
in source:	Cl VDBH 222
Ref:	=2020ApJ...900..138A
by	ASA'D R. , KOVALEV M., DAVIES B., IVANOV V.D., REJKUBA M., GONNEAU A., HERNANDEZ S., LARDO C., BERGEMANN M.
	Astrophys. J., 900, 138-138 (2020)
	Analysis of red supergiants in VDBH 222.
o	Table 1: <[AKD2020] OB22669NN> N=6 among (Nos 28-61).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AKF2009]
[AKF2009]	(Arvidsson+Kerton+Foster, 2009)
Write:	<<[AKF2009] NN>> <<[AKF2009] CTB 102p>>
N:	8
Object:	Filament (SIMBAD class: HIIReg = HII Region)
Note:	100m NRAO Green Bank Telescope radio recombination line observations toward CTB 102.
in source:	CTB 102
Ref:	=2009ApJ...700.1000A
by	ARVIDSSON K. , KERTON C.R., FOSTER T.
	Astrophys. J., 700, 1000-1008 (2009)
	The enormous outer galaxy H II region CTB 102.
o	Tables 1-3: <[AKF2009] NN> N=8 among (Nos 2-10), <[AKF2009] CTB 102p> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AKG2017]
[AKG2017]	(Adams+Kochanek+Gerke+, 2017)
Write:	<<[AKG2017] NNNNN-SFN>> <<[AKG2017] N925-OC1>>
N:	7
Object:	* + SN? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	LBT observations of N=7 failed supernova candidates in N=5 galaxies.
Ref:	=2017MNRAS.469.1445A
by	ADAMS S.M. , KOCHANEK C.S., GERKE J.R., STANEK K.Z.
	Mon. Not. R. Astron. Soc., 469, 1445-1455 (2017)
	The search for failed supernovae with the Large Binocular Telescope: constraints from 7 yr of data.
o	Table 2: <[AKG2017] NNNNN-SFN> N=6, <[AKG2017] N925-OC1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AKH2009]
[AKH2009]	(Aray+Kurtz+Hofner+, 2009)
Write:	<<[AKH2009] DR 21(OH) MM1-WW>> <<[AKH2009] DR 21(OH)-RN>>
N:	2+6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA 0.7cm, 3.6cm, 1.3cm observations of the massive star-forming region DR 21(OH).
in source:	DR 21 (OH)
Ref:	=2009ApJ...698.1321A
by	ARAYA E.D. , KURTZ S., HOFNER P., LINZ H.
	Astrophys. J., 698, 1321-1329 (2009)
	Radio continuum and methanol observations of DR21(OH).
o	Table 3: <[AKH2009] DR 21(OH) MM1-WW> (Nos NW, SE), <[AKH2009] DR 21(OH)-RN> (Nos R1-R6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AKK2003]
[AKK2003]	(Artyukh+Kopylov+Kopylova, 2003)= (PS)
Write:	<<[AKK2003] NNNa>> <<[AKK2003] NNNW>>
N:	260
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Interplanetary scintillating (IPS) radio sources from the Puschino Survey (PS) have been cross-identified with objects from the 7C and FIRST catalogues. In the format, the letter stands for the rank in angular distance: a to f: distance rank for objects within 15', u: unique object within 15' circle, S, W, E: rough direction for objects outside 15' circle.
Ref:	=2003A&A...403..555A
by	ARTYUKH V.S. , KOPYLOV A.I., KOPYLOVA F.G.
	Astron. Astrophys., 403, 555-560 (2003)
	Investigation of radio sources from the interplanetary scintillation Pushchino Survey. I. Cross-identification with the 7C and FIRST radio catalogues.
o	Table 1, cols(7, 8): <[AKK2003] 7C NNNa>, <[AKK2003] 7C NNNW>, N=260. Table 2, col(1, 2, 3): <[AKK2003] FIRST NNNaN>, <[AKK2003] FIRST NNNWN>, N=392.
=E=	Catalogue in electronic form as J/A+A/403/555
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AKM87]
[AKM87]	(Aliakberov+Kononov+Mingaliev+, 1987)
Write:	<<[AKM87] NN>>
N:	72
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Ref:	=1987AISAO..24..178A
by	ALIAKBEROV K.D. , KONONOV V.K., MINGALIEV M.G., NAUGOLNAYA M.N., PLOTNIKOV V.M., PYATUNINA T.B., TRUSHKIN S.A.
	Astrofizik. Issledovanija, 24, 178-182 (1987)
	The flux densities for 72 radio sources in the declination band del=-6 at the wavelength 7.6 cm.
o	Table 1: <[AKM87] NN> (Nos 1-72)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Akn
Akn	(Arakelian)
====>	Equivalent to: Ark
Details on Acronym: [AKN2018]
[AKN2018]	(Akahori +Kato+Nakazawa+, 2018)
Write:	<<[AKN2018] A>>
N:	12
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA 16cm observations of N=12 radio sources in the field of the galaxy cluster CIZA J1358.9-4750.
in source:	CIZA J1358.9-4750
Ref:	=2018PASJ...70...53A
by	AKAHORI T. , KATO Y., NAKAZAWA K., OZAWA T., GU L., TAKIZAWA M., FUJITA Y., NAKANISHI H., OKABE N., MAKISHIMA K.
	PASJ, 70, 53 (2018)
	ATCA 16 cm observation of CIZA J1358.9-4750: Implication of merger stage and constraint on non-thermal properties.
o	Table 2: <[AKN2018] A> (Nos A-L).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AKP89]
[AKP89]	(Anderson+Kulkarni+Prince+, 1989)
Write:	<<[AKP89] M 13 Psr A>>
N:	5
Object:	ms Psr (SIMBAD class: Pulsar)
Stat:	is completely incorporated in Simbad
Note:	Millisecond pulsars in M 13.
in source:	M 13 = NGC 6205
Ref:	=1989IAUC.4819....1A
by	ANDERSON S. , KULKARNI S., PRINCE T., WOLSZCZAN A.
	IAU Circ., 4819, 1-None (1989)
	Ten-millisecond pulsar in M13.
o	First millisecond pulsar discovered in M 13, later designated as pulsar A.
o	<[AKP89] M 13 Psr A> (No. A).
Ref:	=2007ApJ...670..363H
by	HESSELS J.W.T. , RANSOM S.M., STAIRS I.H., KASPI V.M., FREIRE P.C.C.
	Astrophys. J., 670, 363-378 (2007)
	A 1.4 GHz Arecibo survey for pulsars in globular clusters.
o	Tables 3, 4: <[AKP89] M 13 Psr A> (Nos B-E) added, <[WAK89] M 5 Psr A> (Nos C-E) added, <[HRS2007] M 53 Psr A> (No. A), <[HRS2007] M 3 Psr A> (Nos A-D), <[HRS2007] M 71 Psr A> (No. A), <[HRS2007] NGC 6749 Psr A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AKR2004]
[AKR2004]	(Andersen+Knude+Reipurth+, 2004)
Write:	<<[AKR2004] W>>
N:	4
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	SEST observations. Millimetre, optical and NIR observations of M 16 in the vicinity of HH 216. N=4 C18O and CS molecular clouds are observed.
in source:	M 16 = Eagle Nebula = NGC 6611
Ref:	=2004A&A...414..969A
by	ANDERSEN M. , KNUDE J., REIPURTH B., CASTETS A., NYMAN L.A., McCAUGHREAN M.J., HEATHCOTE S.
	Astron. Astrophys., 414, 969-978 (2004)
	Molecular cloud structure and star formation near HH 216 in M 16.
o	Table 1: <[AKR2004] W> (Nos N, C, E, S).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AKR2009]
[AKR2009]	(Angelakis+Kraus+Readhead+, 2009)
Write:	<<[AKR2009] JHHMMSS+DDMM>> <<[AKR2009] HHMMSS+DDMM>> (not recognised by Simbad, but found in literature)
N:	3434
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Effelsberg 100-m telescope 4.85GHz and 10.45GHz observations of N=3434 sources. Use of NVSS data.
Ref:	=2009A&A...501..801A
by	ANGELAKIS E. , KRAUS A., READHEAD A.C.S., ZENSUS J.A., BUSTOS R., KRICHBAUM T.P., WITZEL A., PEARSON T.J.
	Astron. Astrophys., 501, 801-812 (2009)
	Multi-frequency measurements of the NVSS foreground sources in the cosmic background imager fields. I. Data release.
o	Table 8: <[AKR2009] JHHMMSS+DDMM> N=3434.
=E=	Catalogue in electronic form as <J/A+A/501/801/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AKS95]
[AKS95]	(Andruk+Kharchenko+Schilbach+, 1995)= ([AKS95a])
Write:	<<[AKS95] NNNN>>
N:	1141
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1995AN....316..225A
by	ANDRUK V. , KHARCHENKO N., SCHILBACH E., SCHOLZ R.-D.
	Astron. Nachr., 316, 225-248 (1995)
	Photometric survey near the Main Galactic Meridian: 1. Photoelectric stellar magnitudes and colours in the UBVR system.
o	<[AKS95] NNNN> (Nos 1-1141)
=E=	Catalogue in electronic form as J/other/AN/316.225
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AKS95a]
[AKS95a]	(Andruk+Kharchenko+Schilbach+, 1995)
*****	Avoid the usage of [AKS95a], prefer [AKS95]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AKS95b]
[AKS95b]	(Alcala+Krautter+Schmitt+, 1995)
Write:	<<[AKS95b] RX JHHMM.m+DDMMa>>
N:	8
Object:	T Tau * (SIMBAD class: TTauri* = T Tauri Star)
Stat:	is completely incorporated in Simbad
Note:	N=8 WTTS, possible optical counterpart of the corresponding RX J See also [ATW96], [WKS96], [CAA97], [MMS97], [KWS97], [WSK97], [HMC99].
Ref:	=1995A&AS..114..109A
by	ALCALA J.M. , KRAUTTER J., SCHMITT J.H.M.M., COVINO E., WICHMANN R., MUNDT R.
	Astron. Astrophys., Suppl. Ser., 114, 109-134 (1995)
	A study of the Chamaeleon star forming region from the ROSAT all-sky survey. I. X-ray observations and optical identifications.
o	Table 6: <[AKS95b] RX JHHMM.m+DDMMa> N=8
=E=	Catalogue in electronic form as J/A+AS/119/9
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AKU2020]
[AKU2020]	(Akahori+Kitayama+Ueda+, 2020)
Write:	<<[AKU2020] J2344-4243AN>> <<[AKU2020] Source AN>> (not recognised by Simbad, but found in literature)
N:	2+6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ATCA 18GHz observations of N=2+6 radio sources around the brightest galaxy of the Phoenix galaxy cluster.
in source:	SPT-CL J2344-4243 = NAME Phoenix Cluster
Ref:	=2020PASJ...72...62A
by	AKAHORI T. , KITAYAMA T., UEDA S., et al.
	PASJ, 72, 62 (2020)
	Discovery of radio jets in the Phoenix galaxy cluster center.
o	Fig. 1, Table 2: <[AKU2020] J2344-4243AN> (Nos C, W, C1-C6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AKV2001]
[AKV2001]	(Auusteijn+Kuulkers+Van Kerkwijk, 2001) (Not yet in Simbad)
Write:	<<[AKV2001] NN>>
N:	15
Object:	* (SIMBAD class: Star)
Note:	N=15 stars in the field of 4U 1630-47.
Ref:	=2001A&A...375..447A
by	AUGUSTEIJN T. , KUULKERS E., VAN KERKWIJK M.H.
	Astron. Astrophys., 375, 447-454 (2001)
	The IR counterpart of the black-hole candidate 4U1630-47.
o	Table 2, Fig.3: <[AKV2001] NN> (Nos 1-15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AKW99]
[AKW99]	(Aoki+Kosugi+Wilson+, 1999)
Write:	<<[AKW99] NGC 7319 A>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA maps and analyse of HST archival image of NGC 7319. Images in Figs 1, 2.
in source:	NGC 7319
Ref:	=1999ApJ...521..565A
by	AOKI K. , KOSUGI G., WILSON A.S., YOSHIDA M.
	Astrophys. J., 521, 565-571 (1999)
	The radio emission of the Seyfert galaxy NGC 7319.
o	p. 566 Calibrator 2236+284 : 1950 or 2000 coordinates? (= QSO 2234+282 ?)
o	Table 1: <[AKW99] NGC 7319 A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AL
AL	(Andrews+Lindsay)
Write:	<<AL NNN>>
N:	446
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Note:	Often found with the format 'AL-NNN' 3rd list, see also: 1st list: LM 1- and LM 2-, 2nd list: [L63]
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1964IrAJ....6..241A
by	ANDREWS A.D. , LINDSAY E.M.
	Irish Astron. J., 6, 241-247 (1964)
	Third list of emission line objects in the Large Magellanic Cloud.
o	misprint AL 18 = LHA 120-S 65 not LHA 120-S 64
o	<AL NNN> (Nos 1-446)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: AL
AL	(Andrews+Lindsay)
*****	Avoid the usage of AL, prefer [AL67]
Origin	of the Acronym: L (2006ApJ...646L.115O)
Details on Acronym: Al
Al	(Allen)= Ae
Write:	<<PN Al N>> <<PN Al N-A>>
N:	1+19
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Al 1 = PN G006.8-08.6 = PK 006-08 1. 2nd ref.: list 2, format '2-A', (Nos 2-A to 2-S).
Ref:	=1973Obs....93...85A
by	ALLEN D.A.
	The Observatory, 93, 85-85 (1973)
	A new planetary nebula.
o	<PN Al N> (No. 1).
Ref:	=1979Obs....99...83A
by	ALLEN D.A.
	The Observatory, 99, 83-88 (1979)
	On planetary nebulae and Wolf-Rayet stars in the galactic-centre field.
o	Table IV: <PN Al 2-A> (Nos 2-A to 2-S) N=19. Table V: <[A79] N> (Nos 1-2).
Details on Acronym: [AL2000]
[AL2000]	(Aazami+Li+, 2000)
Write:	<<[AL2000] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=1 host galaxy of SN 2000DD
Ref:	=2000IAUC.7477Q...1A
by	AAZAMI A.B. , LI W.D., (The Lick Observatory Supernova Search)
	IAU Circ., 7477, 1-None (2000)
	Supernova 2000dd in anonymous galaxy.
o	<[AL2000] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AL2020]
[AL2020]	(Alp+Larsson, 2020)= ([AL2020a])
Write:	<<[AL2020] XT YYMMDD>> <<[AL2020] XT YYMMDD Host G>>
N:	12+9
Object:	Poss. SN + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=12 SN candidates based on shock breakout (SBO) emission and N=9 host galaxy candidates in the XMM-Newton archive. Use of archival Pan-STARRS, DES, and SkyMapper data.
Ref:	=2020ApJ...896...39A
by	ALP D. , LARSSON J.
	Astrophys. J., 896, 39-39 (2020)
	Blasts from the past: supernova shock breakouts among X-ray transients in the XMM-Newton archive.
o	Fig. 1, Tables 1+3-5+C.1: <[AL2020] XT YYMMDD> N=12. Tables 2+B.1: <[AL2020] XT YYMMDD Host G> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AL2020a]
[AL2020a]	(Alp+Larsson, 2020)
*****	Avoid the usage of [AL2020a], prefer [AL2020]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AL2020b]
[AL2020b]	(Allers+Liu, 2020)= (UHW)
Write:	<<[AL2020b] UHW JDDD.ddddd+DD.ddddd>>
N:	59
Object:	Poss. BD* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	UH88 ULBCam (W filter) observations of N=59 brown dwarf candidates in three star-forming regions (NGC 1333, IC 348, rho Oph).
in source:	NGC 1333
in source:	IC 348
in source:	Name rho Oph Cloud
Ref:	=2020PASP..132j4401A
by	ALLERS K.N. , LIU M.C.
	PASP, 132j, 4401-104401 (2020)
	A novel survey for young substellar objects with the W-band filter. I. Filter design and new discoveries in Ophiuchus and Perseus.
o	Tables 4-6: <[AL2020b] UHW JDDD.ddddd+DD.ddddd> N=59.
=E=	Catalogue in electronic form as <J/PASP/132/J4401/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AL67]
[AL67]	(Andrews+Lindsay)= (AL)
Write:	<<[AL67] Cl* N>> <<[AL67] Neb N>>
N:	5+2
Object:	Cluster of * + Nebula (SIMBAD class: Cluster* = Cluster of Stars)
Note:	New clusters and nebulous objects on ADH plates.
Ref:	=1967IrAJ....8..126A
by	ANDREWS A.D. , LINDSAY E.M.
	Irish Astron. J., 8, 126-None (1967)
	New southern clusters and nebulous ovals.
o	<[AL67] Cl* N> (Nos 1-5). <[AL67] Neb N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AL76]
[AL76]	(Arp+Lorre, 1976)
Write:	<<[AL76] A>>
N:	8
Object:	Feature (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=8 nebulous features between Stephan's Quintet and NGC 7331 region.
Ref:	=1976ApJ...210...58A
by	ARP H. , LORRE J.
	Astrophys. J., 210, 58-64 (1976)
	Image processing of galaxy photographs.
o	Table 1, fig.5: <[AL76] A> (Nos A-H).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AL84]
[AL84]	(Alcaino+Liller, 1984)
Write:	<<[AL84] NGC NNNN A>>
N:	15+24+17+6+10
Object:	* (SIMBAD class: Star)
Note:	Photoelectric UBVRI sequences of stars in the fields of 5 Sculptor galaxies. See also [A81c] for NGC 253.
in source:	NGC 45
in source:	NGC 55
in source:	NGC 247
in source:	NGC 300
in source:	NGC 7793
Ref:	=1984AJ.....89..814A
by	ALCAINO G. , LILLER W.
	Astron. J., 89, 814-818 (1984)
	Photoelectric UBVRI sequences in the Sculptor group galaxies : NGC 45, NGC 55, NGC 247, NGC 253, NGC 300 and NGC 7793.
o	Table VI: [A81c] A stars.
o	Fig.1a, Table III: <[AL84] NGC 45 A> (Nos A-O). Fig.1b, Table IV: <[AL84] NGC 55 A> (Nos A-X). Fig.1c, Table V: <[AL84] NGC 247 A> (Nos A-Q). Fig.1e, Table VII: <[AL84] NGC 300 A> (Nos A-F). Fig.1f, Table VIII: <[AL84] NGC 7793 A> (Nos A-J).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AL87]
[AL87]	(Alcaino+Liller)
Write:	<<[AL87] SL NNN NN>> <<[AL87] NGC NNNN NNN>>
N:	1066
Object:	* (SIMBAD class: Star)
Note:	Las Campanas 2.5m Telescope and La Silla 3.6m telescope observations of star clusters in the Bok region of the LMC.
in source:	NAME LMC
in source:	[SL63] 234
in source:	[SL63] 237
in source:	[SL63] 304
in source:	NGC 1834
in source:	NGC 1836
in source:	NGC 1839
in source:	NGC 1847
in source:	NGC 1850
in source:	NGC 1854
in source:	NGC 1856
in source:	NGC 1858
in source:	NGC 1860
in source:	NGC 1863
in source:	NGC 1870
Ref:	=1987AJ.....94..372A
by	ALCAINO G. , LILLER W.
	Astron. J., 94, 372-402 (1987)
	BVRI photometry of star clusters in the BOK region of the Large Magellanic Cloud.
o	Finding charts
o	Table VIII: <[AL87] NGC 1834 NN> (Nos 1-26). Table X: <[AL87] NGC 1836 NN> (Nos 1-68). Table XII: <[AL87] NGC 1839 NN> (Nos 1-65). Table XIV: <[AL87] NGC 1847 NN> (Nos 1-81). Table XV: <[AL87] NGC 1850 NNN> (Nos 1-217). Table XVII: <[AL87] NGC 1854 NNN> (Nos 1-251). Table XIX: <[AL87] NGC 1856 NNN> (Nos 1-104). Table XX: <[AL87] NGC 1858 NN> (Nos 1-64). Table XXII: <[AL87] NGC 1860 NN> (Nos 1-23). Table XXIII: <[AL87] NGC 1863 NN> (Nos 1-23). Table XXIV: <[AL87] NGC 1870 NN> (Nos 1-22). Table XXV: <[AL87] SL234 NN> (Nos 1-16). Table XXVI: <[AL87] SL 237 NN> (Nos 1-25). Table XXVII: <[AL87] SL304 NN> (Nos 1-81).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ALB2017]
[ALB2017]	(Agnello+Lin+Buckley-Geer+, 2017)
Write:	<<[ALB2017] DES J0408-5354>> <<[ALB2017] DES J0408-5354 AN>> <<[ALB2017] DES J0408-5354 source>>
N:	10+1
Object:	Grav. lens + Grav. lensed image of a QSO + G + QSO (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	ESO/MPG 2.2m telescope WFI and Gemini South GMOS-S observations of N=1 gravitational lens system: N=4 gravitationally lensed images of N=1 QSO, N=6 galaxies including the gravitational lens.
Ref:	=2017MNRAS.472.4038A
by	AGNELLO A. , LIN H., BUCKLEY-GEER L., TREU T., BONVIN V., COURBIN F., LEMON C., MORISHITA T., AMARA A., AUGER M.W., BIRRER S., CHAN J., COLLETT T., MORE A., FASSNACHT C.D., FRIEMAN J., MARSHALL P.J., McMAHON R.G., MEYLAN G., SUYU S.H., CASTANDER F., FINLEY D., HOWELL A., KOCHANEK C., MAKLER M., MARTINI P., MORGAN N., NORD B., OSTROVSKI F., SCHECHTER P., TUCKER D., WECHSLER R., ABBOTT T.M.C., ABDALLA F.B., ALLAM S., BENOIT-LEVY A., BERTIN E., BROOKS D., BURKE D.L., CARNERO ROSELL A., CARRASCO KIND M., CARRETERO J., CROCCE M., CUNHA C.E., D'ANDREA C.B., DA COSTA L.N., DESAI S., DIETRICH J.P., EIFLER T.F., FLAUGHER B., FOSALBA P., GARCIA-BELLIDO J., GAZTANAGA E., GILL M.S., GOLDSTEIN D.A., GRUEN D., GRUENDL R.A., GSCHWEND J., GUTIERREZ G., HONSCHEID K., JAMES D.J., KUEHN K., KUROPATKIN N., LI T.S., LIMA M., MAIA M.A.G., MARCH M., MARSHALL J.L., MELCHIOR P., MENANTEAU F., MIQUEL R., OGANDO R.L.C., PLAZAS A.A., ROMER A.K., SANCHEZ E., SCHINDLER R., SCHUBNELL M., SEVILLA-NOARBE I., SMITH M., SMITH R.C., SOBREIRA F., SUCHYTA E., SWANSON M.E.C., TARLE G., THOMAS D., WALKER A.R.
	Mon. Not. R. Astron. Soc., 472, 4038-4050 (2017)
	Models of the strongly lensed quasar DES J0408-5354.
o	Fig. 2, Table 1: <[ALB2017] DES J0408-5354> N=1, <[ALB2017] DES J0408-5354 AN> (Nos A-D, G1-G5). Text: <[ALB2017] DES J0408-5354 source> N=1.
Ref:	=2017ApJ...838L..15L
by	LIN H. , BUCKLEY-GEER E., AGNELLO A., OSTROVSKI F., McMAHON R.G., NORD B., KUROPATKIN N., TUCKER D.L., TREU T., CHAN J.H.H., SUYU S.H., DIEHL H.T., COLLETT T., GILL M.S.S., MORE A., AMARA A., AUGER M.W., COURBIN F., FASSNACHT C.D., FRIEMAN J., MARSHALL P.J., MEYLAN G., RUSU C.E., ABBOTT T.M.C., ABDALLA F.B., ALLAM S., BANERJI M., BECHTOL K., BENOIT-LEVY A., BERTIN E., BROOKS D., BURKE D.L., CARNERO ROSELL A., CARRASCO KIND M., CARRETERO J., CASTANDER F.J., CROCCE M., D'ANDREA C.B., DA COSTA L.N., DESAI S., DIETRICH J.P., EIFLER T.F., FINLEY D.A., FLAUGHER B., FOSALBA P., GARCIA-BELLIDO J., GAZTANAGA E., GERDES D.W., GOLDSTEIN D.A., GRUEN D., GRUENDL R.A., GSCHWEND J., GUTIERREZ G., HONSCHEID K., JAMES D.J., KUEHN K., LAHAV O., LI T.S., LIMA M., MAIA M.A.G., MARCH M., MARSHALL J.L., MARTINI P., MELCHIOR P., MENANTEAU F., MIQUEL R., OGANDO R.L.C., PLAZAS A.A., ROMER A.K., SANCHEZ E., SCHINDLER R., SCHUBNELL M., SEVILLA-NOARBE I., SMITH M., SMITH R.C., SOBREIRA F., SUCHYTA E., SWANSON M.E.C., TARLE G., THOMAS D., WALKER A.R., (The DES Collaboration)
	Astrophys. J., 838L, 15-15 (2017)
	Discovery of the lensed quasar system DES J0408-5354.
o	Fig. 1, Table 1: <[ALB2017] DES J0408-5354 AN> (No. G0) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ALB2018]
[ALB2018]	(Aguirre+Lindner+Baker+, 2018)
Write:	<<[ALB2018] ACTJHHMM-NNA>>
N:	49+8
Object:	G + (Rad) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	APEX LABOCA 870µm and Australia Telescope Compact Array 2.1GHz observations of N=49 galaxies in 10 galaxy clusters detected through their Sunyaev-Zel'dovich effect (SZE) by the ACT, as part of the Large APEX Bolometer Camera/Atacama Cosmology Telescope (ACT) Survey of Clusters at All Redshifts (LASCAR). Use of archival Herschel PACS and SPIRE and Spitzer IRAC data.
Ref:	=2018ApJ...855...26A
by	AGUIRRE P. , LINDNER R.R., BAKER A.J., BOND J.R., DUNNER R., GALAZ G., GALLARDO P., HILTON M., HUGHES J.P., INFANTE L., LIMA M., MENTEN K.M., SIEVERS J., WEISS A., WOLLACK E.J.
	Astrophys. J., 855, 26-26 (2018)
	The LABOCA/ACT Survey of Clusters at All Redshifts: multiwavelength analysis of background submillimeter galaxies.
o	Tables 5+7-8: <[ALB2018] ACTJHHMM-NNA> N=49+8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ALD2010]
[ALD2010]	(Allers+Liu+Dupuy+, 2010)
Write:	<<[ALD2010] SDSS J2249+0044AB>> <<[ALD2010] SDSS J2249+0044A>>
N:	3
Object:	** + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Keck II NIRC2 LGS AO observations of a young L dwarf binary star.
in source:	SDSS J224953.0+004404.0
Ref:	=2010ApJ...715..561A
by	ALLERS K.N. , LIU M.C., DUPUY T.J., CUSHING M.C.
	Astrophys. J., 715, 561-571 (2010)
	Discovery of a young L dwarf binary, SDSS J224953.47+004404.6AB.
o	<[ALD2010] SDSS J2249+0044AB> N=1, <[ALD2010] SDSS J2249+0044A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ALD2018]
[ALD2018]	(Anthony-Twarog+Lee-Brown+Deliyannis+, 2018) (Not yet in Simbad)
Write:	<<[ALD2018] NNNN>>
N:	135
Object:	* (SIMBAD class: Star)
Note:	WIYN 3.5m telescope HYDRA observations of N=135 stars in NGC 2506, as part of the WIYN open cluster study (WOCS). See also [ADT2016].
in source:	NGC 2506
Ref:	=2018AJ....155..138A
by	ANTHONY-TWAROG B.J. , LEE-BROWN D.B., DELIYANNIS C.P., TWAROG B.A.
	Astron. J., 155, 138-138 (2018)
	WIYN open cluster study. LXXVI. Li evolution among stars of low/intermediate mass: the metal-deficient open cluster NGC 2506.
o	Table 1: <[ALD2018] NNNN> (Nos 7001-7135).
o	Astrometric accuracy is not sufficient for ingestion in Simbad (of the order of 10'')
=E=	Catalogue in electronic form as <J/AJ/155/138/>
Details on Acronym: ALESS
ALESS	(ALMA LABOCA Extended Chandra Deep Field South Submm Survey)
Write:	<<ALESS JHHMMSS.ss+DDMMSS.s>>
N:	about 100
Object:	smm G (SIMBAD class: Galaxy)
Note:	ALMA cycle 0 survey to precisely locate submm sources from the LESS survey (LABOCA Extended Chandra Deep Field South Submm Survey, Weiss et al. 2009ApJ...707.1201W).
in source:	NAME ECDFS
Ref:	=2013ApJ...768...91H
by	HODGE J.A. , KARIM A., SMAIL I., SWINBANK A.M., WALTER F., BIGGS A.D., IVISON R.J., WEISS A., ALEXANDER D.M., BERTOLDI F., BRANDT W.N., CHAPMAN S.C., COPPIN K.E.K., COX P., DANIELSON A.L.R., DANNERBAUER H., DE BREUCK C., DECARLI R., EDGE A.C., GREVE T.R., KNUDSEN K.K., MENTEN K.M., RIX H.-W., SCHINNERER E., SIMPSON J.M., WARDLOW J.L., VAN DER WERF P.
	Astrophys. J., 768, 91 (2013)
	An ALMA survey of submillimeter galaxies in the Extended Chandra Deep Field South: source catalog and multiplicity.
o	Tables 3-4: <[HKS2013] ALESS NNN.NN> = <ALESS JHHMMSS.ss+DDMMSS.s>, N=99+32. Institute for Computational Cosmology, Durham University
=E=	Catalogue in electronic form as <J/ApJ/768/91/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: Alessi
Alessi	(Alessi+)
Write:	<<Cl Alessi NNA>>
Object:	Poss. Stellar Cluster (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Systematic search for unknown star clusters using data included in the Tycho 2 catalogue. Some of the clusters are included in the catalog of clusters in 2002A&A...389..871D.
Ref:	=2003A&A...410..565A
by	ALESSI B.S. , MOITINHO A., DIAS W.S.
	Astron. Astrophys., 410, 565-575 (2003)
	Searching for unknown open clusters in the Tycho-2 catalog.
o	Table 3 : component C of HIP 52436 not in Simbad.
o	Tables 1, 2: <CL Alessi NN> N=11 among (Nos 1-19).
=E=	Catalogue in electronic form as B/ocl
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ALEXIS
ALEXIS	(ALEXIS satellite)
Write:	<<ALEXIS JHHMM+DDd>>
Object:	(EUV) (SIMBAD class: UV = UV-emission Source)
Note:	1st ref. from the ALEXIS satellite. In this ref., N=1 extreme X-ray.
Ref:	=1995IAUC.6152....1R
by	ROUSSEL-DUPRE D. , BLOCH J.J., EDWARDS B.C., PFAFMAN T.E., PRIEDHORSKY W.C., RYAN S., SMITH B.W.
	IAU Circ., 6152, 1-None (1995)
	ALEXIS J1139-685.
o	<ALEXIS JHHMM+DDd> 1st ref. from the ALEXIS satellite survey. In this ref. N=1
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ALF2001]
[ALF2001]	(Alexander+La Franca+Fiore+, 2001)
Write:	<<[ALF2001] NN>> <<[ALF2001] sN>>
N:	11+4
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	BeppoSAX observations. N=11 X-ray sources 'NN', and N=4 supplementary sources 'sN' in the ISO ELAIS S1 region.
Ref:	=2001ApJ...554...18A
by	ALEXANDER D.M. , LA FRANCA F., FIORE F., BARCONS X., CILIEGI P., DANESE L., DELLA CECA R., FRANCESCHINI A., GRUPPIONI C., MATT G., MATUTE I., OLIVER S., POMPILIO F., WOLTER A., EFSTATHIOU A., HERAUDEAU P., PEROLA G.C., PERRI M., RIGOPOULOU D., ROWAN-ROBINSON M.A., SERJEANT S.
	Astrophys. J., 554, 18-26 (2001)
	The European Large-Area Infrared Space Observatory survey V: a BeppoSAX hard X-ray survey of the S1 region.
o	Table 2: <[ALF2001] NN> (Nos 1-11). Table 3: <[ALF2001] sN> (Nos s1-s4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ALFA ZOA
ALFA ZOA	(Arecibo Legacy Fast Zone of Avoidance)
Write:	<<ALFA ZOA JHHMM+DDMM>>
N:	134
Object:	HI G (SIMBAD class: Galaxy)
Note:	Arecibo L-band Feed Array (ALFA) HI observations of galaxies in the Zone of Avoidance (ZOA).
Ref:	=2010AJ....139.2130H
by	HENNING P.A. , SPRINGOB C.M., MINCHIN R.F., MOMJIAN E., CATINELLA B., McINTYRE T., DAY F., MULLER E., KORIBALSKI B., ROSENBERG J.L., SCHNEIDER S., STAVELEY-SMITH L., VAN DRIEL W.
	Astron. J., 139, 2130-2147 (2010)
	The Arecibo L-band Feed Array Zone Of Avoidance survey. I. Precursor observations through the inner and outer Galaxy.
o	Tables 1-2: <ALFA ZOA JHHMM+DDMM> N=72.
Ref:	=2011ApJ...739L..26M
by	McINTYRE T.P. , MINCHIN R.F., MOMJIAN E., HENNING P.A., KAUR A., PARTON B.
	Astrophys. J., 739L, 26 (2011)
	Discovery and follow-up of a nearby galaxy from the Arecibo zone of avoidance survey.
o	<ALFA ZOA JHHMM+DDMM> (No. J1952+1428) added.
Ref:	=2015AJ....150...28M
by	McINTYRE T.P. , HENNING P.A., MINCHIN R.F., MOMJIAN E., BUTCHER Z.
	Astron. J., 150, 28 (2015)
	The ALFA ZOA deep survey: first results.
o	Table 1: <ALFA ZOA JHHMM+DDMM> N=61.
o	C1,C5,C10,C21 and C31 are [ELH2006] CNN in Simbad, but only C5 is in Simbad (no coordinates).
=E=	Catalogue in electronic form as <J/AJ/139/2130/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ALFALFA
ALFALFA	(Arecibo Legacy Fast ALFA)
Write:	<<ALFALFA 1-NNN>> <<ALFALFA 2-NNN>> <<ALFALFA 3-NNN>> <<ALFALFA 4-NNN>> <<ALFALFA 5-NNN>>
N:	730+488+578+541+549
Object:	HI (SIMBAD class: HI = HI (21cm) Source)
Stat.	in SIMBAD: for ALFALFA 1- to ALFALFA 5-
Note:	Arecibo L-band Feed Array (ALFA) receiver system observations of HI regions in the Northern Virgo Cluster, and in the anti-Virgo region at +27deg. See [GHK2005].
in source:	NAME Virgo Cluster
Ref:	=2007AJ....133.2569G
by	GIOVANELLI R. , HAYNES M.P., KENT B.R., SAINTONGE A., STIERWALT S., ALTAF A., BALONEK T., BROSCH N., BROWN S., CATINELLA B., FURNISS A., GOLDSTEIN J., HOFFMAN G.L., KOOPMANN R.A., KORNREICH D.A., MAHMOOD B., MARTIN A.M., MASTERS K.L., MITSCHANG A., MOMJIAN E., NAIR P.H., ROSENBERG J.L., WALSH B.
	Astron. J., 133, 2569-2583 (2007)
	The Arecibo legacy fast ALFA survey. III. H I source catalog of the northern Virgo cluster region.
o	Table 1: <ALFALFA 1-NNN> (Nos 1-1 to 1-730).
Ref:	=2008AJ....135..588S
by	SAINTONGE A. , GIOVANELLI R., HAYNES M.P., HOFFMAN G.L., KENT B.R., MARTIN A.M., STIERWALT S., BROSCH N.
	Astron. J., 135, 588-604 (2008)
	The Arecibo Legacy Fast Alfa Survey. V. The H I source catalog of the Anti-Virgo region at δ = +27°.
o	Table 1: <ALFALFA 2-NNN> (Nos 2-1 to 2-488).
Ref:	=2008AJ....136..713K
by	KENT B.R. , GIOVANELLI R., HAYNES M.P., MARTIN A.M., SAINTONGE A., STIERWALT S., BALONEK T.J., BROSCH N., KOOPMANN R.A.
	Astron. J., 136, 713-724 (2008)
	The Arecibo legacy fast ALFA survey. VI. Second HI source catalog of the Virgo cluster region.
o	WBL 350-005, AGC 213325, AGC 213324 and AGC 221110 not identified.
o	Table 1: <ALFALFA 3-NNN> (Nos 3-1 to 3-578).
Ref:	=2009ApJS..183..214M
by	MARTIN A.M. , GIOVANELLI R., HAYNES M.P., SAINTONGE A., HOFFMAN G.L., KENT B.R., STIERWALT S.
	Astrophys. J., Suppl. Ser., 183, 214-224 (2009)
	The Arecibo Legacy Fast Alfa Survey. VIII. H I source catalog of the anti-Virgo region at δ = +25°.
o	Table 1: <ALFALFA 4-NNN> (Nos 4-1 to 4-541).
Ref:	=2009AJ....138..338S
by	STIERWALT S. , HAYNES M.P., GIOVANELLI R., KENT B.R., MARTIN A.M., SAINTONGE A., KARACHENTSEV I.D., KARACHENTSEVA V.E.
	Astron. J., 138, 338-361 (2009)
	The Arecibo Legacy Fast ALFA Survey. IX. The Leo region H I catalog, group membership, and the H I mass function for the Leo I group.
o	Table 1: <ALFALFA 5-NNN> (Nos 5-1 to 5-549).
=E=	Catalogue in electronic form as J/AJ/133/2569
=E=	Catalogue in electronic form as J/AJ/135/588
=E=	Catalogue in electronic form as J/AJ/136/713
=E=	Catalogue in electronic form as J/ApJS/183/214
=E=	Catalogue in electronic form as <J/AJ/138/338/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ALFALFA
ALFALFA	(Arecibo Legacy Fast ALFA)
*****	Avoid the usage of ALFALFA, prefer [GHK2005]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ALG2015]
[ALG2015]	(Abbas+Layden+Guldenschuh+, 2015)
Write:	<<[ALG2015] NNNN>> <<[ALG2015] VNN>>
N:	1675+13
Object:	* + V* (SIMBAD class: Star)
Note:	CTIO 0.9m telescope and PROMPT4 0.41m telescope observations of N=1675 stars and N=13 variable stars in NGC 6496.
in source:	NGC 6496
Ref:	=2015AJ....149...40A
by	ABBAS M.A. , LAYDEN A.C., GULDENSCHUH K.A., REICHART D.E., IVARSEN K.M., HAISLIP J.B., NYSEWANDER M.C., LACLUYZE A.P., WELCH D.L.
	Astron. J., 149, 40 (2015)
	Variable stars in metal-rich globular clusters. IV. Long-period variables in NGC 6496.
o	Table 2: <[ALG2015] NNNN> N=1675 among (Nos 1-1678). Tables 3-5: <[ALG2015] VNN> (Nos V1-V13).
=E=	Catalogue in electronic form as J/AJ/149/40
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ALH
ALH	(ALHAMBRA)
Write:	<<ALH NNNNNNNNNNN>> <<ALH JHHMMSS+DDMMSS>>
N:	441303+1+352+174
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	The Advance Large Homogeneous Area Medium-Band Astronomical (ALHAMBRA) survey has observed eight different regions of the sky, including sections of the Cosmic Evolution Survey (COSMOS), DEEP2, European Large-Area Infrared Space Observatory Survey (ELAIS), Great Observatories Origins Deep Survey North (GOODS-N), Sloan Digital Sky Survey (SDSS) and Groth fields using a new photometric system with 20 optical, contiguous ∼300-Å filters plus the JHKs bands. Observations were carried out with the 3.5-m telescope at the Calar Alto Observatory (CAHA, Spain), making use of the two wide-field imagers in the optical (LAICA) and NIR (Omega-2000). For more information, visit: http://alhambrasurvey.com 2014MNRAS.441.2891M: The ALHAMBRA gold catalogue corresponds to a subsample of about a thousand galaxies (17<m_F814W<23) with very accurate and reliable photometric redshifts (http://cosmo.iaa.es/content/alhambra-gold-catalog). Format NNNNNNNNNNN: For example, ID = 81442100119 stands for 814 (detection image) + 4 (field) + 2 (pointing) + 1 (CCD) + 00119 (ColorPro_ID).
Ref:	=2013A&A...557A..78M
by	MATUTE I. , MASEGOSA J., MARQUEZ I., FERNANDEZ-SOTO A., HUSILLOS C., DEL OLMO A., PEREA J., POVIC M., ASCASO B., ALFARO E.J., MOLES M., AGUERRI J.A.L., APARICIO-VILLEGAS T., BENITEZ N., BROADHURST T., CABRERA-CANO J., CASTANDER F.J., CEPA J., CERVINO M., CRISTOBAL-HORNILLOS D., INFANTE L., GONZALEZ DELGADO R.M., MARTINEZ V.J., MOLINO A., PRADA F., QUINTANA J.M.
	Astron. Astrophys., 557A, 78-78 (2013)
	The ALHAMBRA survey: discovery of a faint QSO at z = 5.41.
o	<ALH JHHMMSS+DDMMSS> (No. J023002+004647).
Ref:	=2014MNRAS.441.2891M
by	MOLINO A. , BENITEZ N., MOLES M., FERNANDEZ-SOTO A., CRISTOBAL-HORNILLOS D., ASCASO B., JIMENEZ-TEJA Y., SCHOENELL W., ARNALTE-MUR P., POVIC M., COE D., LOPEZ-SANJUAN C., DIAZ-GARCIA L.A., VARELA J., STEFANON M., CENARRO J., MATUTE I., MASEGOSA J., MARQUEZ I., PEREA J., DEL OLMO A., HUSILLOS C., ALFARO E., APARICIO-VILLEGAS T., CERVINO M., HUERTAS-COMPANY M., AGUERRI J.A.L., BROADHURST T., CABRERA-CANO J., CEPA J., GONZALEZ R.M., INFANTE L., MARTINEZ V.J., PRADA F., QUINTANA J.M.
	Mon. Not. R. Astron. Soc., 441, 2891-2922 (2014)
	The ALHAMBRA Survey: Bayesian photometric redshifts with 23 bands for 3 °2.
o	photom.dat: <ALH NNNNNNNNNNN> N=441303 among (Nos 81421100001-81482410419).
Ref:	=2015MNRAS.452..549A
by	ASCASO B. , BENITEZ N., FERNANDEZ-SOTO A., ARNALTE-MUR P., LOPEZ-SANJUAN C., MOLINO A., SCHOENELL W., JIMENEZ-TEJA Y., MERSON A.I., HUERTAS-COMPANY M., DIAZ-GARCIA L.A., MARTINEZ V.J., CENARRO A.J., DUPKE R., MARQUEZ I., MASEGOSA J., NIEVES-SEOANE L., POVIC M., VARELA J., VIIRONEN K., AGUERRI J.A.L., DEL OLMO A., MOLES M., PEREA J., ALFARO E., APARICIO-VILLEGAS T., BROADHURST T., CABRERA-CANO J., CASTANDER F.J., CEPA J., CERVINO M., GONZALEZ DELGADO R.M., CRISTOBAL-HORNILLOS D., HURTADO-GIL L., HUSILLOS C., INFANTE L., PRADA F., QUINTANA J.M.
	Mon. Not. R. Astron. Soc., 452, 549-565 (2015)
	Galaxy clusters and groups in the ALHAMBRA survey.
o	Tables 2-3: <ALH JHHMMSS+DDMMSS> N=352+174.
=E=	Catalogue in electronic form as <J/MNRAS/441/2891/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ALH2005]
[ALH2005]	(Apai+Linz+Henning+, 2005)
Write:	<<[ALH2005] GNN>> <<[ALH2005] SN>> <<[ALH2005] ISN>> <<[ALH2005] A>> <<[ALH2005] NNN>>
N:	15+5+2+9+268
Object:	(Near IR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	ISAAC IR camera at the UT1-VLT of ESO is used to search for Near-IR objects in the field of IRAS 09002-4732. Format 'GNN' for dark Globules, 'SN' for dark filaments, 'ISN' for Isolated Silhouette objects, 'NNN' for NIR. Format 'A' for objects in the vicinity of the HII region GAL 268.42-00.85.
Ref:	=2005A&A...434..987A
by	APAI D. , LINZ H., HENNING T., STECKLUM B.
	Astron. Astrophys., 434, 987-1003 (2005)
	Infrared portrait of the nearby massive star-forming region IRAS 09002-4732.
o	Fig.5, Table 2: <[ALH2005] GNN> (Nos G1-G15), <[ALH2005] SN> (Nos S1-S5), <[ALH2005] ISN> (Nos IS1 , IS2). Fig.12, Table 3: <[ALH2005] A> (Nos A-I). Table 5: <[ALH2005] NNN> (Nos 1-268).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ali
Ali	(Author's name)
Write:	<<** ALI NNNN>>
N:	1192
Object:	(SIMBAD class: = Double or Multiple Star)
Details on Acronym: Alicante
Alicante	(Alicante)
Write:	<<Cl Alicante N>>
N:	2
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Discovery of new stellar clusters.
Ref:	=2008A&A...492..441N
by	NEGUERUELA I. , MARCO A.
	Astron. Astrophys., 492, 441-449 (2008)
	Stellar tracers of the Cygnus Arm. II. A young open cluster in Cam OB3.
o	Wrong coordinates in table 7 for Cl* Alicante 1 NM 217 and Cl* Alicante 1 NM 254
o	Paragr.4.1: <Cl Alicante N> (No. 1). Table 7: <Cl* Alicante 1 NM NNN> N=38 among (Nos 44-695).
Ref:	=2009A&A...493...79M
by	MARCO A. , NEGUERUELA I.
	Astron. Astrophys., 493, 79-88 (2009)
	The open cluster Pismis 11 and the very luminous blue supergiant HD 80077. I. Physical parameters of the cluster.
o	Paragr.2.2: <Cl Alicante N> (No. 5). Table 2: <Cl* Pismis 11 MN NNN> N=145 among (Nos 1-147). Table 5: <Cl* Alicante 5 MN NNN> (Nos 1-105).
=E=	Catalogue in electronic form as <J/A+A/493/79/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ALJ2017]
[ALJ2017]	(An+Lee+Jung+, 2017)
Write:	<<[ALJ2017] NNN>>
N:	712
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	CTIO Blanco 4m telescope Hydra spectroscopy of N=712 stars in ω Centauri. See also Cl* NGC 5139 RLR.
in source:	NGC 5139 = ome Cen
Ref:	=2017AJ....154..150A
by	AN D. , LEE Y.S., JUNG J.I., REY S.-C., RHEE J., LEE J.-W., LEE Y.-W., JOE Y.H.
	Astron. J., 154, 150-150 (2017)
	Medium-resolution spectroscopy of red giant branch stars in ω Centauri.
o	Table 1: <[ALJ2017] NNN> (Nos 1-712).
=E=	Catalogue in electronic form as <J/AJ/154/150/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ALK2018]
[ALK2018]	(Agnello+Lin+Kuropatkin+, 2018)
Write:	<<[ALK2018] WGD JHHMM+DDMM>> <<[ALK2018] WGD JHHMM+DDMM source>> <<[ALK2018] WGD JHHMM+DDMM AN>>
N:	20+9+16+7+3
Object:	Poss. Grav. lens system + QSO + Grav. lensed image of a QSO + Grav. lens + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=20 gravitational lens system candidates selected from a combined search in WISE and Gaia-DR1 over the DES footprint. Magellan 6.5m Baade telescope IMACS follow-up spectroscopy of N=9 background QSOs, N=16 gravitational lensed images of QSOs, N=7 gravitational lenses, and N=3 additional compact sources.
Ref:	=2018MNRAS.479.4345A
by	AGNELLO A. , LIN H., KUROPATKIN N., BUCKLEY-GEER E., ANGUITA T., SCHECHTER P.L., MORISHITA T., MOTTA V., ROJAS K., TREU T., AMARA A., AUGER M.W., COURBIN F., FASSNACHT C.D., FRIEMAN J., MORE A., MARSHALL P.J., McMAHON R.G., MEYLAN G., SUYU S.H., GLAZEBROOK K., MORGAN N., NORD B., ABBOTT T.M.C., ABDALLA F.B., ANNIS J., BECHTOL K., BENOIT-LEVY A., BERTIN E., BERNSTEIN R.A., BROOKS D., BURKE D.L., CARNERO ROSELL A., CARRETERO J., CUNHA C.E., D'ANDREA C.B., DA COSTA L.N., DESAI S., DRLICA-WAGNER A., EIFLER T.F., FLAUGHER B., GARCIA-BELLIDO J., GAZTANAGA E., GERDES D.W., GRUEN D., GRUENDL R.A., GSCHWEND J., GUTIERREZ G., HONSCHEID K., JAMES D.J., KUEHN K., LAHAV O., LIMA M., MAIA M.A.G., MARCH M., MENANTEAU F., MIQUEL R., OGANDO R.L.C., PLAZAS A.A., SANCHEZ E., SCARPINE V., SCHINDLER R., SCHUBNELL M., SEVILLA-NOARBE I., SMITH M., SOARES-SANTOS M., SOBREIRA F., SUCHYTA E., SWANSON M.E.C., TARLE G., TUCKER D., WECHSLER R.
	Mon. Not. R. Astron. Soc., 479, 4345-4354 (2018)
	DES meets Gaia: discovery of strongly lensed quasars from a multiplet search.
o	Table 1: <[ALK2018] WGD JHHMM+DDMM> N=20, <[ALK2018] WGD JHHMM+DDMM source> N=9. Table 2: <[ALK2018] WGD JHHMM+DDMM AN> N=26.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ALL2007]
[ALL2007]	(Alves+ Lombardi+Lada, 2007)
Write:	<<[ALL2007] NNN>>
N:	159
Object:	Dark Cloud (SIMBAD class: MolCld = Molecular Cloud)
Note:	Dense cores in the Pipe Nebula.
in source:	NAME PIPE Nebula
Ref:	=2007A&A...462L..17A
by	ALVES J. , LOMBARDI M., LADA C.J.
	Astron. Astrophys., 462L, 17-21 (2007)
	The mass function of dense molecular cores and the origin of the IMF.
o	Table 1: <[ALL2007] NNN> (Nos 1-159).
=E=	Catalogue in electronic form as J/A+A/462/L17
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ALL76]
[ALL76]	(Abt+Landolt+Levy+, 1976)
Write:	<<[ALL76] A>>
N:	6
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=6 stars in gamma Vel group (possible physical association). Map Fig.1.
Ref:	=1976AJ.....81..541A
by	ABT H.A. , LANDOLT A.U., LEVY S.G., MOCHNACKI S.
	Astron. J., 81, 541-543 (1976)
	Visual multiples. II. The γ Velorum group.
o	Table 1: <[ALL76] A> (Nos A-F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AllWISE
AllWISE	(AllWISE Source Catalog)
*****	Avoid the usage of AllWISE, prefer WISEA
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [ALM2000]
[ALM2000]	(Afanas'ev+Lozinskaya+Moiseev+, 2000) (Not yet in Simbad)
Write:	<<[ALM2000] N>>
N:	3
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Fig.2: N=3 compact features in the region of the bright core S3 = [S71b] HII 3, in IC 1613. No. 1 = WO star = [AM85] IC 1613 3.
in source:	IC 1613
Ref:	=2000AstL...26..153A
by	AFANAS'EV V.L. , LOZINSKAYA T.A., MOISEEV A.V., BLANTON E.
	Astron. Lett., 26, 153-161 (2000)
	A giant bipolar shell around the WO star in the galaxy IC 1613: structure and kinematics.
o	WO star = [AM85] IC 1613 3.
o	Fig.2: <[ALM2000] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ALM2001]
[ALM2001]	(Augereau+Lagrange+Mouillet+, 2001)
Write:	<<[ALM2001] HD 100546 A>>
N:	3
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	HST/NICMOS2 observations. N=3 brightest companion stars in the vicinity of HD 100546.
Ref:	=2001A&A...365...78A
by	AUGEREAU J.-C. , LAGRANGE A.-M., MOUILLET D., MENARD F.
	Astron. Astrophys., 365, 78-89 (2001)
	HST/NICMOS2 coronagraphic observations of the circumstellar environment of three old PMS stars: HD 100546, SAO 206462 and MWC 480.
o	close binary near SAO 206462 not in SIMBAD.
o	Table 3, Fig.1: <[ALM2001] HD 100546 A> (Nos B, C, D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ALM2007]
[ALM2007]	(Allen+Luhman+Myers+, 2007)= (IRAC)
Write:	<<[ALM2007] IRAC JHHMMSSss+DDMMSSs>>
N:	5
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC observations of the Lupus 3 cloud.
in source:	Lupus 3
Ref:	=2007ApJ...655.1095A
by	ALLEN P.R. , LUHMAN K.L., MYERS P.C., MEGEATH S.T., ALLEN L.E., HARTMANN L., FAZIO G.G.
	Astrophys. J., 655, 1095-1102 (2007)
	New low-mass stars and brown dwarfs with disks in Lupus.
o	Table 3: <[ALM2007] IRAC JHHMMSSss+DDMMSSs> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ALMA
ALMA	(The Atacama Large Millimeter/submillimeter Array)
Write:	<<ALMA JHHMMSS.s+DDMMSS>> <<ALMA JHHMMSS.ss+DDMMSS.s>> <<ALMA JHHMMSS.sss+DDMMSS.ss>> <<ALMA JHHMMSS.ssss+DDMMSS.sss>>
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	We propose here a designator for newly discovered sources by ALMA. Due to the nature of ALMA with very large variability in resolution, depending on the configuration of the telescope, we suggest here – after having contacted Francois Ochsenbein (http://cdsweb.u-strasbg.fr/Dic/iau-spec.html) – to allow ALMA source designations with different precisions. This allows to separate sources at high resolution without having to resort to additional letters as well as having to add random numbers to the names. The proposed naming scheme has been approved by ALMA's Head of Science Operations.
Notes:	There exist already a number of ALMA publications, that have studied ALMA background sources and some have used already their own. http://arxiv.org/pdf/1508.05099 ALMACAL J130349.05.554034.2 http://arxiv.org/pdf/1508.00644 ALMA SXDS1 13015 1 http://arxiv.org/pdf/1505.03523 http://arxiv.org/pdf/1502.00640 http://arxiv.org/pdf/1403.4360 http://arxiv.org/pdf/1304.6437
Auth.:	Felix Stoehr ESO/ALMA
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: ALMACAL
ALMACAL	(ALMA Calibration)
Write:	<<ALMACAL JHHMMSS.ss+DDMMSS.s>> <<ALMACAL HHMMSS.ss+DDMMSS.s>> (not recognised by Simbad, but found in literature)
N:	52
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Continuum detections, as part of the submillimeter survey ALMACAL, using ALMA calibration observations to detect and study high-redshift dusty, star-forming galaxies (DSFGs). For more information, visit: https://almacal.wordpress.com/ 2016ApJ...822...36O: N=13 DSFGs and N=1 likely jet 2020MNRAS.495.2332K: N=38 (21 DSFGs, 7 potential jets, and 10 jets)
Ref:	=2016ApJ...822...36O
by	OTEO I. , ZWAAN M.A., IVISON R.J., SMAIL I., BIGGS A.D.
	Astrophys. J., 822, 36-36 (2016)
	ALMACAL I: first dual-band number counts from a deep and wide ALMA submillimeter survey, free from cosmic variance.
o	Table 2+Text: <ALMACAL JHHMMSS.ss+DDMMSS.s> N=13+1.
Ref:	=2020MNRAS.495.2332K
by	KLITSCH A. , ZWAAN M.A., SMAIL I., PEROUX C., BIGGS A.D., CHEN C.-C., IVISON R.J., POPPING G., LAGOS C., BETHERMIN M., SWINBANK A.M., HAMANOWICZ A., DUTTA R.
	Mon. Not. R. Astron. Soc., 495, 2332-2341 (2020)
	ALMACAL VII: first interferometric number counts at 650 µm.
o	Table 1: <ALMACAL JHHMMSS.ss+DDMMSS.s> N=38.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ALP
ALP	(Anguita+Loyola+Pedreros)
*****	Avoid the usage of ALP, prefer [ALP2000]
Origin	of the Acronym: L (2002AJ....123.1971P)
Details on Acronym: [ALP2000]
[ALP2000]	(Anguita+Loyola+Pedreros, 2000)= (ALP)
Write:	<<[ALP2000] JHHMM+DDMM>> <<[ALP2000] JHHMM+DDMM NN>>
N:	2+23+52+16
Object:	QSO + * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=2 QSOs behind the LMC, from Maza, 1989, private communication. Tables 2-4: N=23 ref. stars in the field of QSO [VV98c] J055721.8-671338. N=52 ref. stars in the field of QSO [ALP2000] J0558-6707. N=16 ref. stars in the field of QSO [ALP2000] J0615-6615. See also [PAM2002].
Ref:	=2000AJ....120..845A
by	ANGUITA C. , LOYOLA P., PEDREROS M.H.
	Astron. J., 120, 845-854 (2000)
	Proper motion of the Large Magellanic Cloud using QSOs as an inertial reference system.
o	Table 1: <[ALP2000] JHHMM+DDMM> N=2. Tables 2-4: <[ALP2000] JHHMM+DDMM NN> N=23+52+16.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ALR-GC C
ALR-GC C	(Azzopardi+Lequeux+Rebeirot, Gal. Center, Carbon *)
Write:	<<ALR-GC C NN>>
N:	34
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Note:	1st results evocated by Azzopardi et al. in 1985A&A...145L...4A with an ALR provisional number (obsolete) Finding Charts
in source:	NAME Galactic Bulge
Ref:	=1991A&AS...88..265A
by	AZZOPARDI M. , LEQUEUX J., REBEIROT E., WESTERLUND B.E.
	Astron. Astrophys., Suppl. Ser., 88, 265-275 (1991)
	Carbon stars in the galactic bulge-identification, spectrophotometric and infrared photometric data.
o	Table 2: <ALR-GC C NN> (Nos 1-34)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ALS
ALS	(Alma Luminous Star)
Write:	<<ALS NNNNN>>
N:	5132+7390
Object:	Star (SIMBAD class: Star)
Note:	(Nos 1-5132) are identical to 'LS NNNN' Southern stars (Nos 5133-6000) are not assigned (Nos 6001-13390) are Northern LS stars, cross-id. with 'LS R +DD NNN' are not given in 1998ApJS..115..271R.
Ref:	=1998ApJS..115..271R
by	REED B.C.
	Astrophys. J., Suppl. Ser., 115, 271-276 (1998)
	UBV β database for Case-Hamburg Northern and Southern Luminous Stars.
o	Many wrong crossids
o	<ALS NNNNN> (Nos 1-5132, 6001-13390)
Ref:	=2003AJ....125.2531R
by	REED B.C.
	Astron. J., 125, 2531-2533 (2003)
	Catalog of galactic OB stars.
o	Catalog: <ALS NNNNN> N=6171 among (Nos 14001-20171) added.
=E=	Catalogue in electronic form as J/ApJS/115/271
=E=	Catalogue in electronic form as V/125
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ALS
ALS	(Acker+Lundstrom+Stenholm)
*****	Avoid the usage of ALS, prefer [ALS88]
Origin	of the Acronym: L (1997A&A...327..191M)
Details on Acronym: [ALS82]
[ALS82]	(Aaronson+Liebert+Stocke, 1982)= (Dra) = (Draco)
Write:	<<[ALS82] CN>>
N:	3
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Note:	In the format, the letter 'C' stands for Carbon * [ALS82] C1 to C3 are respectively = to McClure C1 to C3
in source:	NAME Draco Dwarf Galaxy
Ref:	=1982ApJ...254..507A
by	AARONSON M. , LIEBERT J., STOCKE J.
	Astrophys. J., 254, 507-514 (1982)
	Discovery of carbon stars in the Draco dwarf spheroidal galaxy.
o	Table 1: <[ALS82] CN> (Nos C1-C3)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ALS88]
[ALS88]	(Acker+Lundstrom+Stenholm, 1988)= (ALS)
Write:	<<[ALS88] N>>
N:	2
Object:	Symb. * (SIMBAD class: Symbiotic* = Symbiotic Star)
Stat:	is completely incorporated in Simbad
Note:	N=2 symbiotic stars
Ref:	=1988A&AS...73..325A
by	ACKER A. , LUNDSTROM I., STENHOLM B.
	Astron. Astrophys., Suppl. Ser., 73, 325-333 (1988)
	Spectrophotometry of new symbiotic stars.
o	Table I: <[ALS88] N> (Nos 1-2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Alter
Alter	(Author's name)
Write:	<<Cl Alter N>>
N:	1
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Stat:	is completely incorporated in Simbad
Details on Acronym: ALW
ALW	(Azzopardi+Lequeux+Westerlund)
Write:	<<ALW Sculptor N>> <<ALW Carina NN>> <<ALW Leo II N>> <<ALW Leo I NN>>
N:	8+12+7+20
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Note:	C* in Scl Dw. G: format 'Sculptor N', N=8 C* in Car Dw. G: format 'Carina NN', N=12 C* in Leo II Dw. G: format 'Leo II N', N=7 C* in Leo I Dw. G: format I NN', N=20
in source:	NAME SDIG
in source:	NAME Carina Dwarf Galaxy
in source:	UGC 6253 = Leo II
in source:	UGC 5470 = Leo I
Ref:	=1985A&A...144..388A
by	AZZOPARDI M. , LEQUEUX J., WESTERLUND B.E.
	Astron. Astrophys., 144, 388-394 (1985)
	New carbon stars in spheroidal galaxies. I. Sculptor, Carina, Leo I and Leo II systems.
o	Table 2: <ALW Sculptor N> N=6. Table 3: <ALW Carina NN> N=11. Table 4: <ALW Leo II N> N=7
Ref:	=1986A&A...161..232A
by	AZZOPARDI M. , LEQUEUX J., WESTERLUND B.E.
	Astron. Astrophys., 161, 232-236 (1986)
	New carbon stars in spheroidal galaxies. II. Draco, Ursa Minor and new data on Sculptor, Carina and Leo I.
o	Table 2: <ALW Sculptor N> N=8. Table 3: <ALW Carina NN> N=12. Table 4: <ALW Leo I NN> N=19
Ref:	=1989ApJ...345..759Z
by	ZARITSKY D. , OLSZEWSKI E.W., SCHOMMER R.A., PETERSON R.C., AARONSON M.
	Astrophys. J., 345, 759-769 (1989)
	Velocities of stars in remote galactic satellites and the mass of the galaxy.
o	<ALW Leo I NN> No. 20 added
Origin	of the Acronym: L = Found in the literature
Details on Acronym: AM
AM	(Arp+Madore)= APM
Write:	<<AM HHMM+DDM>> <<AM HHMM+DDMM>>
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	In the format the declination is not 'DDd' but 'DDM'. The authors have truncated the arc minutes instead of writing a decimal fraction of degree: e.g. +43deg 59' is written +435. Vol.I. Positions and descriptions. Vol. II. Selected photographs (photographic reproductions by W.E. Roberton)
Ref:	=1987AM....C......0A
by	ARP H.C. , MADORE B.F.
	Cambridge Univ. Press, 0-None (1987)
	A catalogue of southern peculiar galaxies and associations.
o	<AM HHMM+DDM>
=E=	Catalogue in electronic form as VII/170
Details on Acronym: AM
AM	(Armandroff+Massey)
*****	Avoid the usage of AM, prefer [AM85]
Origin	of the Acronym: L (1998ApJ...505..793M)
Details on Acronym: AM
AM	(Arp+Madore)
Write:	<<Cl AM N>>
N:	4
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	Cl AM 1 = NAME E 1 = ESO 201-SC10, intergalactic, galactocentric distance 118 kpc (Aaronson+, 1984, Ap. J. 276, 221-228 and plates 1 and 2) Cl AM 2 = ESO 368-SC07 Cl AM 3 probably belongs to the SMC Cl AM 4 = C 1353-269, probably intergalactic
Ref:	=1979ApJ...227L.103M
by	MADORE B.F. , ARP H.C.
	Astrophys. J., 227, 103-104 (1979)
	Three new faint star clusters.
o	<Cl AM N> (Nos 1-3)
Ref:	=1982PASP...94...40M
by	MADORE B.F. , ARP H.C.
	Publ. Astron. Soc. Pac., 94, 40-42 (1982)
	A distant star cluster in Hydra, AM-4.
o	<Cl AM N> No. 4
Details on Acronym: [AM2002]
[AM2002]	(Adami+Mazure, 2002)
Write:	<<[AM2002] DDD.dddd+DD.dddd>>
N:	80
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Format built on RA and Dec in degrees.
Ref:	=2002A&A...381..420A
by	ADAMI C. , MAZURE A.
	Astron. Astrophys., 381, 420-427 (2002)
	Group analysis in the SSRS2 catalog.
o	Tables 1, 2: <[AM2002] DDD.dddd+DD.dddd> N=80.
=E=	Catalogue in electronic form as J/A+A/381/420
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AM2011]
[AM2011]	(Andreon+Moretti, 2011)
Write:	<<[AM2011] NN>>
N:	43
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	Swift X-Ray Telescope archival data of N=43 optically selected clusters of galaxies. Use of the maxBCG cluster catalog (see [KMA2007]).
Ref:	=2011A&A...536A..37A
by	ANDREON S. , MORETTI A.
	Astron. Astrophys., 536A, 37-37 (2011)
	Do X-ray dark or underluminous galaxy clusters exist?
o	Tables 1-2: <[AM2011] NN> (Nos 1-43).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AM77]
[AM77]	(Ardeberg+Maurice, 1977)= (AM) = (ArM) = (ArMa) = (SMC ArM)
Write:	<<[AM77] NN>>
N:	92
Object:	Superg. (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Same authors and same year in ref. 1977A&AS...28..153A: see [ArMa].
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1977A&AS...30..261A
by	ARDEBERG A. , MAURICE E.
	Astron. Astrophys., Suppl. Ser., 30, 261-278 (1977)
	Observations of supergiant stars in the Small Magellanic Cloud.
o	Acronym ArMa not used for this ref. in SIMBAD, but [AM77]. ArMa is used for ref. 1977A&AS...28..153A.
o	Catalogue: <[AM77] NN> (Nos 1-92)
=E=	Catalogue in electronic form as J/A+AS/30/261
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AM85]
[AM85]	(Armandroff+Massey, 1985)= (AM) = (WR)
Write:	<<[AM85] NGC 6822 NN>> <<[AM85] IC 1613 N>> <<[AM85] M 33 NN>>
N:	12+8+27
Object:	Poss. WR (SIMBAD class: WolfRayet* = Wolf-Rayet)
Note:	Table 4: format 'NGC 6822 NN', N=12 WR candidates in NGC 6822 Table 4: format 'IC 1613 N' N=8, WR candidates in IC 1613 Table 5: format 'M 33 NN', N=27 WR candidates in M 33.
in source:	NGC 6822
in source:	IC 1613
in source:	M 33 = NGC 598
Ref:	=1985ApJ...291..685A
by	ARMANDROFF T.E. , MASSEY P.
	Astrophys. J., 291, 685-692 (1985)
	Wolf-Rayet stars in NGC 6822 and IC 1613.
o	Table 4: <[AM85] NGC 6822 NN> N=12, <[AM85] IC 1613 N> N=8. Table 5: <[AM85] M 33 NN> N=27
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AM93]
[AM93]	(Appleton+Marcum, 1993)
Write:	<<[AM93] N>> <<[AM93] A>> <<[AM93] a>>
N:	8+2+2
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Table 1: format 'N' (Nos 1-8) are knots format 'A' (Nos A-B) are nucleus components format 'a' (Nos a-b) are HII regions
in source:	NGC 985
Ref:	=1993ApJ...417...90A
by	APPLETON P.N. , MARCUM P.M.
	Astrophys. J., 417, 90-96 (1993)
	Infrared observations of the Seyfert ring galaxy NGC 985.
o	Table 1: <[AM93] N> (Nos 1-8), <[AM93] a> (Nos a-b), <[AM93] A> (Nos A-B)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMA2008]
[AMA2008]	(Ascaso+Moles+Aguerri+, 2009)
Write:	<<[AMA2008] ANNNN JHHMMSS.ss+DDMMSS.s>>
N:	408
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	NOT observations of five clusters of galaxies.
in source:	ACO 2658
in source:	ACO 1643
in source:	ACO 1878
in source:	ACO 2111
in source:	ACO 1952
Ref:	=2008A&A...487..453A
by	ASCASO B. , MOLES M., AGUERRI J.A.L., SANCHEZ-JANSSEN R., VARELA J.
	Astron. Astrophys., 487, 453-460 (2008)
	The bright galaxy population of five medium redshift clusters. I. Color-magnitude relation, blue fractions, and visual morphology.
o	Table A: <[AMA2008] ANNNN JHHMMSS.ss+DDMMSS.s> N=408.
=E=	Catalogue in electronic form as <J/A+A/487/453/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMA2011]
[AMA2011]	(Atlee+Martini+Assef+, 2011)
Write:	<<[AMA2011] aNNNN NNN>> <<[AMA2011] ms1008 NNN>> <<[AMA2011] ac114 NNN>>
N:	580
Object:	G (SIMBAD class: Galaxy)
Note:	Las Campanas Observatory 2.5m du Pont telescope and Spitzer IRAC and MIPS observations of N=8 galaxy clusters.
in source:	ACO 3128
in source:	ACO 3125
in source:	ACO 644
in source:	ACO 2104
in source:	ACO 1689
in source:	ACO 2163
in source:	1E 1008.0-1224
in source:	ACCG 114
Ref:	=2011ApJ...729...22A
by	ATLEE D.W. , MARTINI P., ASSEF R.J., KELSON D.D., MULCHAEY J.S.
	Astrophys. J., 729, 22 (2011)
	A multi-wavelength study of low-redshift clusters of galaxies. I. Comparison of X-ray and mid-infrared selected active galactic nuclei.
o	Tables 2-3: <[AMA2011] aNNNN NNN> N=362, <[AMA2011] ms1008 NNN> (Nos 001-096), <[AMA2011] ac114 NNN> (Nos 001-202).
=E=	Catalogue in electronic form as J/ApJ/729/22
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMB2011]
[AMB2011]	(Azimlu+Marciniak+Barmby, 2011)
Write:	<<[AMB2011] HII NNNN>> <<[AMB2011] NNN>>
N:	3961+407
Object:	HII + Em. Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Mayall 4m telescope observations of N=3961 HII regions and N=407 potential PNe in M31.
in source:	M 31 = NGC 224
Ref:	=2011AJ....142..139A
by	AZIMLU M. , MARCINIAK R., BARMBY P.
	Astron. J., 142, 139 (2011)
	A new catalog of H II regions in M31.
o	Table 2: <[AMB2011] HII NNNN> (Nos 1-3961). Table 3: <[AMB2011] NNN> (Nos 1-407).
=E=	Catalogue in electronic form as J/AJ/142/139
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMB2013]
[AMB2013]	(Alves De Oliveira+Moraux+Bouvier+, 2013)
Write:	<<[AMB2013] CFHT-IC 348 NN>>
N:	31
Object:	Poss. Brown Dwarf (SIMBAD class: BrownD*_Candidate = Brown Dwarf Candidate)
Note:	CFHT MegaCam and WIRCam photometry and GTC Osiris and Gemini GNIRS spectroscopic observations of N=31 candidates in the nearby star cluster IC 348.
in source:	IC 348
Ref:	=2013A&A...549A.123A
by	ALVES DE OLIVEIRA C. , MORAUX E., BOUVIER J., DUCHENE G., BOUY H., MASCHBERGER T., HUDELOT P.
	Astron. Astrophys., 549A, 123-123 (2013)
	Spectroscopy of brown dwarf candidates in IC 348 and the determination of its substellar IMF down to planetary masses.
o	Table 2: <[AMB2013] CFHT-IC 348 NN> N=31.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMB96]
[AMB96]	(Asselin+Menard+Bastien+, 1996)
Write:	<<[AMB96] A>>
N:	7
Object:	Feature (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Fig.4a: features in the V376 Cas nebulosity, labeled (Nos A-D) Fig.8: features surrounding V633 Cas, labeled (Nos E-G) See also [CRB95]
Ref:	=1996ApJ...472..349A
by	ASSELIN L. , MENARD F., BASTIEN P., MONIN J.-L., ROUAN D.
	Astrophys. J., 472, 349-359 (1996)
	The environment of V633 Cassiopeiae and V376 Cassiopeiae: evidence for circumstellar disks.
o	<HH NNN> (Nos 162, 164). Figs 4a, 8: <[AMB96] A> (Nos A-G)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMC2015]
[AMC2015]	(Adams+Martini+Croxall+, 2015)
Write:	<<[AMC2015] LBG4 N>> <<[AMC2015] LBG4E N>> <<[AMC2015] FILL NN>>
N:	15+11
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	LBT MODS spectroscopy of N=15+11 Lyman-break galaxies (LBGs) around luminous z∼4 QSOs.
Ref:	=2015MNRAS.448.1335A
by	ADAMS S.M. , MARTINI P., CROXALL K.V., OVERZIER R.A., SILVERMAN J.D.
	Mon. Not. R. Astron. Soc., 448, 1335-1344 (2015)
	Discovery of an overdensity of Lyman α emitters around a z ~ 4 QSO with the Large Binocular Telescope.
o	Table 3: <[AMC2015] LBG4 N> (Nos LBG4 1 to LBG4 8), <[AMC2015] LBG4E N (Nos LBG4E 1 to LBG4E 7). Table 4: <[AMC2015] FILL NN> (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMD2002]
[AMD2002]	(Allen+Myers+Di Francesco+, 2002)
Write:	<<[AMD2002] JHHMMSS+DDMMSSA>>
N:	163
Object:	* (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	HST NICMOS3 observations. Near-IR photometry of young stars associated with the rho Oph molecular cloud.
in source:	NAME rho Oph Cloud
Ref:	=2002ApJ...566..993A
by	ALLEN L.E. , MYERS P.C., DI FRANCESCO J., MATHIEU R., CHEN H., YOUNG E.
	Astrophys. J., 566, 993-1004 (2002)
	Hubble space Telescope/NICMOS imaging survey of the Ophiuchus (Lynds 1688) cluster.
o	Tables 2, 3: <[AMD2002] JHHMMSS+DDMMSSA> N=163.
=E=	Catalogue in electronic form as J/ApJ/566/993
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AMDM
AMDM	(Andre+Martin-Pintado+Despois+Montmerle)= (VLA)
Write:	<<AMDM VLA HHMM.m+DDMM>> <<AMDM Blue N>> <<AMDM Red N>>
N:	1+4+3
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	VLA and IRAM observations (1990A&A...236..180A), JCMT observations (1995MNRAS.277..193D). rho Oph cloud. The probable driving source is designated as 'VLA 1623.4-2418' often found in the literature as 'VLA 1623' (NAME VLA 1623 in SIMBAD).
in source:	NAME rho Oph Cloud
Ref:	=1990A&A...236..180A
by	ANDRE P. , MARTIN-PINTADO J., DESPOIS D., MONTMERLE T.
	Astron. Astrophys., 236, 180-192 (1990)
	Discovery of a remarkable bipolar flow and exciting source in the ρ Ophiuchi cloud core.
o	Text: <AMDM VLA 1623.4-2418> = <NAME VLA 1623>. Fig.2, Tables 1: <AMDM Blue N> (Nos 1-3), <AMDM Red N> (Nos 1-3).
Ref:	=1995MNRAS.277..193D
by	DENT W.R.F. , MATTHEWS H.E., WALTHER D.M.
	Mon. Not. R. Astron. Soc., 277, 193-209 (1995)
	CO and shocked H2 in the highly collimated outflow from VLA 1623.
o	Text: <AMDM Blue N> (No. 4) added. Fig.6, Table 2: <[DMW95] AN> (Nos H1-H8).
Origin	of the Acronym: L (1995MNRAS.277..193D)
Details on Acronym: [AMF99]
[AMF99]	(Antonello+Mantegazza+Fugazza+, 1999)
Write:	<<[AMF99] VNNNN>>
N:	113
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	See also [AFM2000], [AFM2002], [AFM2002b].
in source:	IC 1613
Ref:	=1999A&A...349...55A
by	ANTONELLO E. , MANTEGAZZA L., FUGAZZA D., BOSSI M., COVINO S.
	Astron. Astrophys., 349, 55-69 (1999)
	Variable stars in nearby galaxies. I. Search for Cepheids in field A of IC 1613.
o	T.3: SV NN = [S71b] VNN.
o	Tables 4-7: <[AMF99] VNNNN> N=43+22+8+38 among (Nos 33-3106).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMG2008]
[AMG2008]	(Andre+Minier+Gallais+, 2008)
Write:	<<[AMG2008] SN-AN>>
N:	7
Object:	Core (SIMBAD class: denseCore = Dense Core)
Note:	APEX P-Artemis 450mu.m observations of the NGC 3576 region. See also [PML2009].
Ref:	=2008A&A...490L..27A
by	ANDRE P. , MINIER V., GALLAIS P., REVERET V., LE PENNEC J., RODRIGUEZ L., BOULADE O., DOUMAYROU E., DUBREUIL D., LORTHOLARY M., MARTIGNAC J., TALVARD M., DE BREUCK C., HAMON G., SCHNEIDER N., BONTEMPS S., LAGAGE P.O., PANTIN E., ROUSSEL H., MILLER M., PURCELL C.R., HILL T., STUTZKI J.
	Astron. Astrophys., 490L, 27-30 (2008)
	First 450 µm dust continuum mapping of the massive star-forming region NGC 3576 with the P-ArTeMiS bolometer camera.
o	Fig. 1, Tables 1-2: <[AMG2008] SN-AN> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMH2017]
[AMH2017]	(Ao+Matsuda+Henkel+, 2017)
Write:	<<[AMH2017] ALMA-LABNNa>> <<[AMH2017] VLA-LABNNa>>
N:	10+20
Object:	Lyman Alpha Blob + (smm) + (Rad) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	JCMT-SCUBA2, ALMA band 7, and VLA observations of 35 Lymanα blobs (LABs, see [MYH2004]) at z∼3.1 in the SSA 22 field.
in source:	SSA 22
Ref:	=2017ApJ...850..178A
by	AO Y. , MATSUDA Y., HENKEL C., IONO D., ALEXANDER D.M., CHAPMAN S.C., GEACH J., HATSUKADE B., HAYES M., HINE N.K., KATO Y., KAWABE R., KOHNO K., KUBO M., LEHNERT M., MALKAN M., MENTEN K.M., NAGAO T., NORRIS R.P., OUCHI M., SAITO T., TAMURA Y., TANIGUCHI Y., UMEHATA H., WEISS A.
	Astrophys. J., 850, 178-178 (2017)
	Deep submillimeter and radio observations in the SSA22 field. I. Powering sources and the Lyα escape fraction of Lyα blobs.
o	Table 2, col(1): <[AMH2017] ALMA-LABNNa> (Nos 1-2, 5, 12, 14, 18, 18a-18d). Table 2, col(8): <[AMH2017] VLA-LABNNa> (Nos 1a-1b, 2-3, 4a-4b, 5, 9a-9b, 11, 14, 16, 18a-18b, 18d, 30a-30d).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMI2005]
[AMI2005]	(Adami+Mazure+Ilbert+, 2005)
Write:	<<[AMI2005] NN>> <<[AMI2005] NN-N>>
N:	17+6
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	VIMOS VLT deep survey combined with other surveys from literature to detect several galaxy structures in the CDFS. N=17 compact structures are found, Structure 9 is a diffuse wall including one compact structure (9-1), Structure 11 is a compact wall split in 5 smaller structures (11-1 to 11-5).
in source:	NAME CDFS
Ref:	=2005A&A...443..805A
by	ADAMI C. , MAZURE A., ILBERT O., CAPPI A., BOTTINI D., GARILLI B., LE BRUN V., LE FEVRE O., MACCAGNI D., PICAT J.P., SCARAMELLA R., SCODEGGIO M., TRESSE L., VETTOLANI G., ZANICHELLI A., ARNABOLDI M., ARNOUTS S., BARDELLI S., BOLZONELLA M., CHARLOT S., CILIEGI P., CONTINI T., COVONE G., FOUCAUD S., FRANZETTI P., GAVIGNAUD I., GUZZO L., IOVINO A., LAUGER S., McCRACKEN H.J., MARANO B., MARINONI C., MENEUX B., MERIGHI R., PALTANI S., PELLO R., POLLO A., POZZETTI L., RADOVICH M., ZAMORANI G., ZUCCA E., BONDI M., BONGIORNO A., BUSARELLO G., GREGORINI L., MATHEZ G., MELLIER Y., MERLUZZI P., RIPEPI V., RIZZO D.
	Astron. Astrophys., 443, 805-818 (2005)
	The Vimos VLT Deep Survey: compact structures in the CDFS.
o	Table 4: <[AMI2005] NN> (Nos 1-17). Table 5: <[AMI2005] NN-N> (Nos 9-1, 11-1 to 11-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AMI2011
AMI2011	(AMI Consortium, 2011)= (AMI2011a)
Write:	<<AMI2011 IRAM 04191 N>> <<AMI2011 LNNNNA N>> <<AMI2011 L673-7 N>> <<AMI2011 B35A NN>> <<AMI2011 CB188 1>> <<AMI2011 BERN 48 1>>
N:	47
Object:	Radio(cm) (SIMBAD class: cmRad = Centimetric Radio Source)
Note:	AMI Large Array 1.8cm observations of N=47 sources towards 13 protostellar regions selected from the Spitzer c2d small clouds and cores programme.
Ref:	=2011MNRAS.410.2662S
by	SCAIFE A.M.M. , CURTIS E.I., DAVIES M., FRANZEN T.M.O., GRAINGE K.J.B., HOBSON M.P., HURLEY-WALKER N., LASENBY A.N., OLAMAIE M., POOLEY G.G., RODRIGUEZ-GONZALVEZ C., SAUNDERS R.D.E., SCHAMMEL M., SCOTT P.F., SHIMWELL T., TITTERINGTON D., WALDRAM E., ZWART J.T.L.
	Mon. Not. R. Astron. Soc., 410, 2662-2678 (2011)
	AMI Large Array radio continuum observations of Spitzer c2d small clouds and cores AMI consortium:.
o	Table 4: <AMI2011 IRAM 04191 N> (Nos 1-2), <AMI2011 LNNNNA N> N=32, <AMI2011 L637-7 N> (Nos 1-2), <AMI2011 B35A NN> (Nos 1-11), <AMI2011 CB188 1>, <AMI2011 BERN 48 1>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AMI2011a
AMI2011a	(AMI Consortium, 2011) (Not yet in Simbad)
*****	Avoid the usage of AMI2011a, prefer AMI2011
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AMI2011b
AMI2011b	(AMI Consortium, 2011)
Write:	<<AMI2011b PLCKESZ GLLL.ll+BB.bb A>>
N:	19+19
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	AMI Large Array (LA) and Small Array (SA) observations of N=19+19 in the fields of PLCKESZ G115.71+17.52 and PLCKESZ G121.11+57.01, respectively.
in source:	PLCKESZ G115.71+17.52
in source:	PLCKESZ G121.11+57.01
Ref:	=2011MNRAS.414L..75H
by	HURLEY-WALKER N. , BROWN M.L., DAVIES M.L., FEROZ F., FRANZEN T.M.O., GRAINGE K., HOBSON M.P., LASENBY A., OLAMAIE M., POOLEY G., RODRIGUEZ-GONZALVEZ C., SAUNDERS R.D.E., SCHAMMEL M.P., SCAIFE A.M.M., SCOTT P.F., SHIMWELL T., TITTERINGTON D., WALDRAM E., (The AMI Consortium)
	Mon. Not. R. Astron. Soc., 414L, 75-79 (2011)
	Further Sunyaev–Zel'dovich observations of two Planck ERCSC clusters with the Arcminute Microkelvin Imager.
o	Fig. 1, Tables 3-4: <AMI2011b PLCKESZ GLLL.ll+BB.bb A> N=19+19.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AMI2012
AMI2012	(AMI Consortium, 2012)= (AMI2012a)
Write:	<<AMI2012 ANNNN A>>
N:	14+14+12+9+18+15
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	AMI observations of N=82 radio sources in the field of six galaxy clusters.
Ref:	=2012MNRAS.419.2921A
by	AMI CONSORTIUM , HURLEY-WALKER N., BRIDLE S., CYPRIANO E.S., DAVIES M.L., ERBEN T., FEROZ F., FRANZEN T.M.O., GRAINGE K., HOBSON M.P., LASENBY A., MARSHALL P.J., OLAMAIE M., POOLEY G., RODRIGUEZ-GONZALVEZ C., SAUNDERS R.D.E., SCAIFE A.M.M., SCHAMMEL M.P., SCOTT P.F., SHIMWELL T., TITTERINGTON D., WALDRAM E., ZWART J.T.L.
	Mon. Not. R. Astron. Soc., 419, 2921-2942 (2012)
	Bayesian analysis of weak gravitational lensing and Sunyaev-Zel'dovich data for six galaxy clusters.
o	Figs 5-10, Tables A1-A6: <AMI2012 ANNNN A> N=14+14+12+9+18+15.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AMI2012a
AMI2012a	(AMI Consortium+, 2012)
*****	Avoid the usage of AMI2012a, prefer AMI2012
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AMI2012b
AMI2012b	(AMI Consortium+, 2012)
Write:	<<AMI2012b AMI NN>> <<AMI2012b JHHMMSS.ss+DDMMSS.s>> <<AMI2012b AMI-NN>> (not recognised by Simbad, but found in literature)
N:	14+39
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	AMI Large Array 1.8cm observations of cores identified as deeply embedded young stellar objects in the Serpens molecular cloud.
in source:	NAME Serpens Cloud
Ref:	=2012MNRAS.420.1019A
by	AMI CONSORTIUM , SCAIFE A.M.M., HATCHELL J., AINSWORTH R.E., BUCKLE J.V., DAVIES M., FRANZEN T.M.O., GRAINGE K.J.B., HOBSON M.P., HURLEY-WALKER N., LASENBY A.N., OLAMAIE M., PERROTT Y.C., POOLEY G.G., RICHER J.S., RODRIGUEZ-GONZALVEZ C., SAUNDERS R.D.E., SCHAMMEL M.P., SCOTT P.F., SHIMWELL T., TITTERINGTON D., WALDRAM E.
	Mon. Not. R. Astron. Soc., 420, 1019-1033 (2012)
	AMI-LA radio continuum observations of Spitzer c2d small clouds and cores: Serpens region.
o	Tables 4-6, col(1): <AMI2012b AMI NN> (Nos 1-14). Tables 4-5: <AMI2012b JHHMMSS.ss+DDMMSS.s> N=25+3. Tables 5-6: <AMI2012b JHHMMSS.s+DDMMSS> N=9, <AMI2012b JHHMMSS.s+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AMI2012c
AMI2012c	(AMI Consortium, 2012)= ([SBB2012])
Write:	<<AMI2012c JHHMMSS.ss+DDMMSS.ss>> <<AMI2012c JHHMMSS.s+DDMMSS.s>>
N:	18
Object:	(Radio) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	AMI (Arcminute Microkelvin Imager) observations of N=18 galaxy cluster candidates in the AMI002 field.
Ref:	=2012MNRAS.423.1463A
by	AMI CONSORTIUM , SHIMWELL T.W., BARKER R.W., BIDDULPH P., BLY D., BOYSEN R.C., BROWN A.R., BROWN M.L., CLEMENTSON C., CROFTS M., CULVERHOUSE T.L., CZERES J., DACE R.J., DAVIES M.L., D'ALESSANDRO R., DOHERTY P., DUGGAN K., ELY J.A., FELVUS M., FEROZ F., FLYNN W., FRANZEN T.M.O., GEISBUSCH J., GENOVA-SANTOS R., GRAINGE K.J.B., GRAINGER W.F., HAMMETT D., HOBSON M.P., HOLLER C.M., HURLEY-WALKER N., JILLEY R., KANEKO T., KNEISSL R., LANCASTER K., LASENBY A.N., MARSHALL P.J., NEWTON F., NORRIS O., NORTHROP I., ODELL D.M., OLAMAIE M., PERROTT Y.C., POBER J.C., POOLEY G.G., POSPIESZALSKI M.W., QUY V., RODRIGUEZ-GONZALVEZ C., SAUNDERS R.D.E., SCAIFE A.M.M., SCHAMMEL M.P., SCHOFIELD J., SCOTT P.F., SHAW C., SMITH H., TITTERINGTON D.J., VELIC M., WALDRAM E.M., WEST S., WOOD B.A., YASSIN G., ZWART J.T.L.
	Mon. Not. R. Astron. Soc., 423, 1463-1473 (2012)
	A blind detection of a large, complex, Sunyaev-Zel'dovich structure.
o	Table 5: <AMI2012c JHHMMSS.ss+DDMMSS.ss> N=16. Fig. 6, Paragr. 5: <AMI2012c JHHMMSS.s+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AMI2012d
AMI2012d	(AMI Consortium, 2012)
Write:	<<AMI2012d ANNNNa N>> <<AMI2012d RXJHHMM+DDMM N>> <<AMI2012d ZwHHMM.m+DDMM N>>
N:	72
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	AMI 16GHz interferometric observations of N=72 sources in 19 clusters from the LoCuSS survey and of ACO 1758S.
Ref:	=2012MNRAS.425..162R
by	RODRIGUEZ-GONZALVEZ C. , SHIMWELL T.W., DAVIES M.L., FEROZ F., FRANZEN T.M.O., GRAINGE K.J.B., HOBSON M.P., HURLEY-WALKER N., LASENBY A.N., OLAMAIE M., POOLEY G., SAUNDERS R.D.E., SCAIFE A.M.M., SCHAMMEL M.P., SCOTT P.F., TITTERINGTON D.J., WALDRAM E.M.
	Mon. Not. R. Astron. Soc., 425, 162-203 (2012)
	Detailed Sunyaev–Zel'dovich study with AMI of 19 LoCuSS galaxy clusters: masses and temperatures out to the virial radius.
o	Table 5: <AMI2012d ANNNNa N>, <AMI2012d RXJHHMM+DDMM N>, <AMI2012d ZwHHMM.m+DDMM N>, N=72.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AMIGPS
AMIGPS	(AMI Galactic Plane Survey)
Write:	<<AMIGPS JHHMMSS+DDMMSS>>
N:	3503
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	AMI SA 15.7GHz observations of N=3503 (first data release) sources, as part of the AMI Galactic Plane Survey.
Ref:	=2013MNRAS.429.3330P
by	PERROTT Y.C. , SCAIFE A.M.M., GREEN D.A., DAVIES M.L., FRANZEN T.M.O., GRAINGE K.J.B., HOBSON M.P., HURLEY-WALKER N., LASENBY A.N., OLAMAIE M., POOLEY G.G., RODRIGUEZ-GONZALVEZ C., RUMSEY C., SAUNDERS R.D.E., SCHAMMEL M.P., SCOTT P.F., SHIMWELL T.W., TITTERINGTON D.J., WALDRAM E.M., (The AMI Consortium)
	Mon. Not. R. Astron. Soc., 429, 3330-3340 (2013)
	AMI Galactic Plane Survey at 16 GHz - I. Observing, mapping and source extraction.
o	The AMIGPS catalog available from CDS list the right ascension with 2 decimals more than the excerpt given in the table 4 (thanks to the author).
o	<AMIGPS JHHMMSS+DDMMSS> N=3503.
=E=	Catalogue in electronic form as J/MNRAS/429/3330
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AMK2006]
[AMK2006]	(Afonso+Mobasher+Koekemoer+, 2006)
Write:	<<[AMK2006] NNa>>
N:	72
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Optical and X-ray identifications of 64 radio sources in the CDF-S of the GOODS survey. See also ATCDFS.
in source:	NAME CDFS
Ref:	=2006AJ....131.1216A
by	AFONSO J. , MOBASHER B., KOEKEMOER A., NORRIS R.P., CRAM L.
	Astron. J., 131, 1216-1230 (2006)
	Optical and X-ray identification of faint radio sources in the GOODS CDF-S Advanced Camera for Surveys field.
o	Table 1: <[AMK2006] NNa> N=72 (Nos 1-64) = <ATCDFS JHHMMSS.ss+DDMMSS.s> N=64.
=E=	Catalogue in electronic form as J/AJ/131/1216
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMK2008]
[AMK2008]	(Akiyama+Minowa+Kobayashi+, 2008)
Write:	<<[AMK2008] QHHMM+DDd-AANNNNA>> <<[AMK2008] QHHMM+DDMM-AANNNNA>> <<[AMK2008] DSF2237b-AANNA>> <<[AMK2008] QHHMM+DDd-N-AONNN>> <<[AMK2008] QHHMM+DDMM-N-AONNN>> <<[AMK2008] DSF2237b-N-AONNN>> <<[AMK2008] 4C 28.58A>>
N:	13+4+4+3+2
Object:	Knot + Distant Red G (SIMBAD class: Galaxy)
Note:	Subaru AO-assisted NIR observations of Lyman-Break Galaxies (LBG) and Distant Red Galaxies (DRG).
in source:	SAS-LBG Q0302-MD373
in source:	SAS-LBG Q0302-M80
in source:	SAS-LBG Q0302-MD216
in source:	SAS-LBG Q0302-D73
in source:	SAS-LBG Q2233-MD46
in source:	SAS-LBG DSF2237b-MD90
in source:	SAS-LBG DSF2237b-MD13
in source:	4C 28.58
Ref:	=2008ApJS..175....1A
by	AKIYAMA M. , MINOWA Y., KOBAYASHI N., OHTA K., ANDO M., IWATA I.
	Astrophys. J., Suppl. Ser., 175, 1-28 (2008)
	Adaptive optics rest-frame v-band imaging of Lyman break galaxies at z~3: high surface density disklike galaxies?.
o	Table 6, Fig.5: <[AMK2008] Q0302-003-AANNNNA> N=3+2+2+2, <[AMK2008] Q2233+1341-AANNNNA> N=2, <[AMK2008] DSF2237b-AANNA> N=2+2. Table 7: <[AMK2008] Q0302-003-N-AONNN> N=3, <[AMK2008] Q2233+1341-N-AONNN> N=1, <[AMK2008] DSF2237b-N-AONNN> N=3, <[AMK2008] 4C 28.58A> (Nos 28.58A, 28.58B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMM2003]
[AMM2003]	(Albacete Colombo+Mendez+Morrell, 2003)
Write:	<<[AMM2003] NN>>
N:	80
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of the Carina Nebula.
in source:	Carina Nebula = NGC 3372
Ref:	=2003MNRAS.346..704A
by	ALBACETE COLOMBO J.F. , MENDEZ M., MORRELL N.I.
	Mon. Not. R. Astron. Soc., 346, 704-718 (2003)
	XMM-Newton X-ray observations of the Carina nebula.
o	in ref list CHEN 1991ApJ...366..512C instead of ApJ.336.512, SEWARD 197 9ApJ...234L..55S instead of ApJ.234.55
o	Table 2: <[AMM2003] NN> (Nos 1-80).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMM2009]
[AMM2009]	(Ammons+Melbourne+Max+, 2009)= ([AMM2009a])
Write:	<<[AMM2009] NormN>> <<[AMM2009] Normal N>> (not recognised by Simbad, but found in literature)
N:	9
Object:	G (SIMBAD class: Galaxy)
Note:	Keck II NIRC2 AO observations of galaxies in the GOODS South field. Use of archival HST ACS GOODS data. N=9 objects in a comparative sample.
in source:	NAME GOODS South Field
Ref:	=2009AJ....137..470A
by	AMMONS S.M. , MELBOURNE J., MAX C.E., KOO D.C., ROSARIO D.J.V.
	Astron. J., 137, 470-497 (2009)
	Spatially resolved stellar populations of eight GOODS-South active galactic nuclei at z ~ 1.
o	Table 2: <[AMM2009] NormN> (Nos Norm1 to Norm9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMM2009a]
[AMM2009a]	(Ammons+Melbourne+Max+, 2009)
*****	Avoid the usage of [AMM2009a], prefer [AMM2009]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMM2009b]
[AMM2009b]	(Arnold+Martini+Maulchaey+, 2009)
Write:	<<[AMM2009b] JHHMMSS.s+DDMMSS.s>> <<[AMM2009b] JHHMMSS.ss+DDMMSS.s>>
N:	12+1
Object:	X AGN (SIMBAD class: AGN = Active Galaxy Nucleus)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of X-ray AGN in X-ray selected groups and clusters of galaxies.
Ref:	=2009ApJ...707.1691A
by	ARNOLD T.J. , MARTINI P., MULCHAEY J.S., BERTI A., JELTEMA T.E.
	Astrophys. J., 707, 1691-1706 (2009)
	Active galactic nuclei in groups and clusters of galaxies: detection and host morphology.
o	Fig. 3, Table 4: <[AMM2009b] JHHMMSS.s+DDMMSS.s> N=12, <[AMM2009b] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMN2018]
[AMN2018]	(Alonso-Santiago+Marco+Negueruela+, 2018)
Write:	<<[AMN2018] NNN>>
N:	607
Object:	* (SIMBAD class: Star)
Note:	ESO NTT 3.6m telescope EFOSC2 photometry and SAAO 1.9m telescope spectroscopy of N=607 stars in the open cluster NGC 3105.
in source:	NGC 3105
Ref:	=2018A&A...616A.124A
by	ALONSO-SANTIAGO J. , MARCO A., NEGUERUELA I., TABERNERO H.M., CASTRO N., McBRIDE V.A., RAJOELIMANANA A.F.
	Astron. Astrophys., 616A, 124-124 (2018)
	NGC 3105: a young open cluster with low metallicity.
o	Table A.1: <[AMN2018] NNN> (Nos 1-607).
=E=	Catalogue in electronic form as J/A+A/616/A124
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMO2006]
[AMO2006]	(Andersen+Meyer+Oppenheimer+, 2006)
Write:	<<[AMO2006] NNN>>
N:	181
Object:	* in Cl* (SIMBAD class: Star)
Note:	HST NICMOS images of the cluster associated with Mon R2.
in source:	NAME Mon R2 Cluster
Ref:	=2006AJ....132.2296A
by	ANDERSEN M. , MEYER M.R., OPPENHEIMER B., DOUGADOS C., CARPENTER J.
	Astron. J., 132, 2296-2308 (2006)
	NICMOS2 Hubble space telescope observations of the embedded cluster associated with Mon R2: constraining the substellar initial mass function.
o	Table 2: <[AMO2006] NNN> (Nos 1-181).
=E=	Catalogue in electronic form as J/AJ/132/2296
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMO2014]
[AMO2014]	(Anderson+Meier+Ott+, 2014)
Write:	<<[AMO2014] NN>>
N:	13
Object:	Clump (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	ATCA HCN(1-0) and HCO+(1-0) observations of the dense gas in the star-forming region 30 Doradus.
in source:	Magellanic Clouds:LMC:30 Dor Nebula = 30 Dor Nebula
in source:	Magellanic Clouds:LMC:[JGB98] 30 Dor-10 = [JGB98] 30 Dor-10
Ref:	=2014ApJ...793...37A
by	ANDERSON C.N. , MEIER D.S., OTT J., HUGHES A., WONG T., HENKEL C., CHEN R., INDEBETOUW R., LOONEY L., MULLER E., PINEDA J.L., SEALE J.
	Astrophys. J., 793, 37 (2014)
	From gas to stars in energetic environments: dense gas clumps in the 30 Doradus region within the Large Magellanic Cloud.
o	Fig. 1, Table 1: <[AMO2014] NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMP2004]
[AMP2004]	(Argo+Muxlow+Pedlar+, 2004)= ([AMP2004a])
Write:	<<[AMP2004] JHHMMSS+DDMMSS>>
N:	1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA and MERLIN observations of NGC 3310. Discovery of a variable compact steep spectrum source. of NGC 3310.
in source:	NGC 3310
Ref:	=2004MNRAS.351L..66A
by	ARGO M.K. , MUXLOW T.W.B., PEDLAR A., BESWICK R.J., STRONG M.
	Mon. Not. R. Astron. Soc., 351, 66-70 (2004)
	A possible radio supernova in the outer part of NGC 3310.
o	<[AMP2004] JHHMMSS+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMP2004a]
[AMP2004a]	(Argo+Muxlow+Pedlar+, 2004)
*****	Avoid the usage of [AMP2004a], prefer [AMP2004]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMP2004b]
[AMP2004b]	(Amram+Mendes de Oliveira+Plana+, 2004) (Not yet in Simbad)
Write:	<<[AMP2004b] AN>>
N:	2
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Two objects are seen in the Fabry-Perot velocity maps of the HCG 31 group, objects A1 and A2 east of the complex HCG 31a + HCG 31c.
in source:	HCG 31
Ref:	=2004ApJ...612L...5A
by	AMRAM P. , MENDES DE OLIVEIRA C., PLANA H., BALKOWSKI C., HERNANDEZ O., CARIGNAN C., CYPRIANO E.S., SODRE L.Jr, GACH J.L., BOULESTEIX J.
	Astrophys. J., 612, 5-8 (2004)
	The compact group of galaxies HCG 31 in an early phase of merging.
o	Fig.1: <[AMP2004b] AN> (Nos A1-A2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMP2005]
[AMP2005]	(Asif+Mundell+Pedlar, 2005) (Not yet in Simbad)
Write:	<<[AMP2005] NGC 4151 WW>> <<[AMP2005] NGC 4151 WWN>>
N:	2+4
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	XMM-Newton observations of NGC 4151: N=2 HII regions (Nos NW, SE), and in each region: 2 dislocated arcs NW1-NW2, and each side of an omega-like ridge SE1-SE2.
in source:	NGC 4151
Ref:	=2005MNRAS.359..408A
by	ASIF M.W. , MUNDELL C.G., PEDLAR A.
	Mon. Not. R. Astron. Soc., 359, 408-416 (2005)
	Kinematics of ionized gas in the barred Seyfert galaxy NGC 4151.
o	Text: <[AMP2005] NGC 4151 WW> (Nos NW, SE), <[AMP2005] NGC 4151 WWN> (Nos NW1-NW2, SE1-SE2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMP2011]
[AMP2011]	(Adami+Mazure+Pierre+, 2011)
Write:	<<[AMP2011] JHHMMSS.s+DDMMSS>> <<[AMP2011] C555>> <<[AMP2011] DD.ddd+DD.ddd>>
N:	7+1+11
Object:	Cluster of G + Poss. Group of G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Search for clusters of galaxies in the XMM-LSS survey.
Ref:	=2011A&A...526A..18A
by	ADAMI C. , MAZURE A., PIERRE M., SPRIMONT P.G., LIBBRECHT C., PACAUD F., CLERC N., SADIBEKOVA T., SURDEJ J., ALTIERI B., DUC P.A., GALAZ G., GUEGUEN A., GUENNOU L., HERTLING G., ILBERT O., LE FEVRE J.P., QUINTANA H., VALTCHANOV I., WILLIS J.P., AKIYAMA M., AUSSEL H., CHIAPPETTI L., DETAL A., GARILLI B., LEBRUN V., LEFEVRE O., MACCAGNI D., MELIN J.B., PONMAN T.J., RICCI D., TRESSE L.
	Astron. Astrophys., 526A, 18-18 (2011)
	The XMM-LSS survey: optical assessment and properties of different X-ray selected cluster classes.
o	Tables 2-5: <XLSSC NNN> N=56 among (Nos 000-070). Table 4: <[AMP2011] C555> N=1. Table 5: <[AMP2011] JHHMMSS.s+DDMMSS> N=7. Table B.1: <[AMP2011] DDD.ddd+DD.ddd> N=11.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMP2019]
[AMP2019]	(Araya+Mitchell+Parsons, 2019)
Write:	<<[AMP2019] JHHMMSS.s+DDMMSS.s>>
N:	3
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	N=3 gamma-ray point sources near HESS J1825-137. Use of Fermi LAT data.
Ref:	=2019MNRAS.485.1001A
by	ARAYA M. , MITCHELL A.M.W., PARSONS R.D.
	Mon. Not. R. Astron. Soc., 485, 1001-1007 (2019)
	Revealing a new region of γ-ray emission in the vicinity of HESS J1825-137.
o	Fig. 3: <[AMP2019] JHHMMSS.s+DDMMSS.s> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMR2003]
[AMR2003]	(Arnal+May+Romero, 2003)
Write:	<<[AMR2003] A>>
N:	16
Object:	CO em. feature (SIMBAD class: PartofCloud = Part of Cloud)
Note:	CO molecular features toward OB association Ara OB1.
in source:	NAME ASS ARA OB 1-
Ref:	=2003A&A...412..431A
by	ARNAL E.M. , MAY J., ROMERO G.A.
	Astron. Astrophys., 412, 431-445 (2003)
	A ^{12}CO (J = 1 -> 0) study towards the Ara OB1 region.
o	Fig.4, Table 1: <[AMR2003] A> (Nos A-P).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMR2018]
[AMR2018]	(Araujo de Souza+Martins+Rodriguez-Ardila+, 2018)
Write:	<<[AMR2018] NNN>>
N:	976
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	SOAR SAM observations of N=976 HII regions in NGC 1232.
in source:	NGC 1232
Ref:	=2018AJ....155..234A
by	ARAUJO DE SOUZA A. , MARTINS L.P., RODRIGUEZ-ARDILA A., FRAGA L.
	Astron. J., 155, 234-234 (2018)
	Star formation rate distribution in the galaxy NGC 1232.
o	Fig. 2, Table 1: <[AMR2018] NNN> (Nos 1-976).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMR93]
[AMR93]	(Arnal+Morras+Rizzo, 1993)
Write:	<<[AMR93] NN>>
N:	56
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1993MNRAS.265....1A
by	ARNAL E.M. , MORRAS R., RIZZO J.R.
	Mon. Not. R. Astron. Soc., 265, 1-11 (1993)
	Multicolour polarization and CO observations towards a dark filament in Musca.
o	<[AMR93] NN> N=56
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AMS
AMS	(Alejo Martinez-Sansigre)
Write:	<<AMS NN>>
N:	21
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	N=21 QSOs from the Spitzer FLS radio catalogue.
Ref:	=2005Natur.436..666M
by	MARTINEZ-SANSIGRE A. , RAWLINGS S., LACY M., FADDA D., MARLEAU F.R., SIMPSON C., WILLOTT C.J., JARVIS M.J.
	Nature, 436, 666-669 (2005)
	The obscuration by dust of most of the growth of supermassive black holes.
o	ref.18: 2003AJ....125.2411C (not ApJ)
o	Table 1: <AMS NN> (Nos 1-21).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AMS2000]
[AMS2000]	(Arnaud+Maurogordato+Slezak+, 2000)
Write:	<<[AMS2000] XW>> <<[AMS2000] A521W>> <<[AMS2000] JHHMMSS.s+DDMMSS.s>> <<[AMS2000] gN>> <<[AMS2000] gA>> <<[AMS2000] NN>>
N:	2+2+9+3+1+20
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI images of ACO 521. N=2 X-ray peaks (Nos XN, XS), corresponding to the two sub-clusters (Nos A521N, A521S). Table 1, col(6, 7): N=9 proposed optical counterparts to RX sources, format 'JHHMMSS.s+DDMMSS.s'. In Figs 8 and 10, galaxies are found in the field of ACO 521: (Nos g1-g3) and (No. gA). Table A1: N=20 radio-sources (NVSS) in the field of ACO 521.
in source:	ACO 521
Ref:	=2000A&A...355..461A
by	ARNAUD M. , MAUROGORDATO S., SLEZAK E., RHO J.
	Astron. Astrophys., 355, 461-478 (2000)
	A521: A cluster forming at the crossing of two filaments?
o	Optical ridges of galaxies S1 and S2 are not objects in SIMBAD.
o	Text: <[AMS2000] XW> (Nos XN, XS), <[AMS2000] A521W> (Nos A521N, A521S). Table 1, col(6, 7): <[AMS2000] JHHMMSS.s+DDMMSS.s> N=9. Fig.8: <[AMS2000] gN> (Nos g1-g3). Fig.10: <[AMS2000] gA> (No. gA). Table A1: <[AMS2000] NN> (Nos 1-20).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMS2018]
[AMS2018]	(Amodeo+Mei+Stanford+, 2018)
Write:	<<[AMS2018] PLCK GLLL.ll+BB.bb>> <<[AMS2018] PLCK GLLL.ll+BB.bb NN>> <<[AMS2018] PSZ2 GLLL.ll+BB.bb NN>>
N:	23+412
Object:	Cluster of G + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Keck LRIS and Gemini GMOS spectroscopic observations of N=412 galaxies in 53 Planck clusters (including N=23 with format PLCK GLLL.ll+BB.bb).
Ref:	=2018ApJ...853...36A
by	AMODEO S. , MEI S., STANFORD S.A., LAWRENCE C.R., BARTLETT J.G., STERN D., CHARY R.-R., SHIM H., MARLEAU F.R., MELIN J.-B., RODRIGUEZ-GONZALVEZ C.
	Astrophys. J., 853, 36-36 (2018)
	Spectroscopic confirmation and velocity dispersions for 20 Planck galaxy clusters at 0.16 < z < 0.78.
o	Table 4: <[AMS2018] PLCK GLLL.ll+BB.bb> N=23. Table 5: <[AMS2018] PLCK GLLL.ll+BB.bb NN> , <[AMS2018] PSZ2 GLLL.ll+BB.bb NN> N=412.
=E=	Catalogue in electronic form as <J/ApJ/853/36/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMT2006]
[AMT2006]	(Ajiki+Mobasher+tANIGUCHI+, 2006)
Write:	<<[AMT2006] NN>>
N:	14
Object:	LAE (SIMBAD class: EmObj = Emission Object)
Stat:	is completely incorporated in Simbad
Note:	Subaru Suprime-Cam observations of the GOODS fields: LAE candidates with z about 5.7, (Nos 1-10) in GOODS North field and (Nos 11-14) in GOODS South field.
in source:	NAME GOODS North Field
in source:	NAME GOODS South Field
Ref:	=2006ApJ...638..596A
by	AJIKI M. , MOBASHER B., TANIGUCHI Y., SHIOYA Y., NAGAO T., MURAYAMA T., SASAKI S.S.
	Astrophys. J., 638, 596-602 (2006)
	Narrowband survey of the GOODS fields: search for Lyα emitters at z = 5.7.
o	Table 1, Fig.2: <[AMT2006] NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMY2001]
[AMY2001]	(Aoyama+Mizuno+Yamamoto+, 2001) (Not yet in Simbad)
Write:	<<[AMY2001] C18O NN>> <<[AMY2001] H13CO+ NN>>
N:	19+11
Object:	Clump (SIMBAD class: Cloud)
Note:	N=18 C18O clumps and N=11 H13CO+ clumps in Ori B region.
in source:	NAME Ori B
Ref:	=2001PASJ...53.1053A
by	AOYAMA H. , MIZUNO N., YAMAMOTO H., ONISHI T., MIZUNO A., FUKUI Y.
	Publ. Astron. Soc. Jap., 53, 1053-1062 (2001)
	A large-scale study of H13CO+ and CO18O (J=1 – 0) in Orion B.
o	Table 1: <[AMY2001] C18O NN> (Nos 1-19). Table 2: <[AMY2001] H13CO+ NN> (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AMZ99]
[AMZ99]	(Alonso+Minniti+Zijlstra+, 1999)
Write:	<<[AMZ99] NN>>
N:	65
Object:	* (SIMBAD class: Star)
Note:	IR photometry of NGC 3109. N=65 stars.
in source:	NGC 3109
Ref:	=1999A&A...346...33A
by	ALONSO M.V. , MINNITI D., ZIJLSTRA A.A., TOLSTOY E.
	Astron. Astrophys., 346, 33-44 (1999)
	Infrared photometry of the inner regions of the dwarf irregular galaxy NGC 3109.
o	Table 3: <[AMZ99] NN> (Nos 1-65).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: An
An	(Anonymous)
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Auth.:	PFLEIDERER J.+
*****	Avoid the usage of An, prefer An Cl
Details on Acronym: AN
AN	(Astronomische Nachrichten)
Write:	<<AN NNN.YYYY>>
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Rem:	V* Nomenclature.
=E=	Catalogue in electronic form as IV/23
Details on Acronym: An
An	(Anonymous)
*****	Avoid the usage of An, prefer [GG70]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: An
An	(Anonymous)
*****	Avoid the usage of An, prefer ZHT
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: An 1 XRS
An 1 XRS	(X-ray source, list 1)
*****	Avoid the usage of An 1 XRS, prefer 1XRS
Details on Acronym: An 2 XRS
An 2 XRS	(X-ray source, list 2) (Not yet in Simbad)
*****	Avoid the usage of An 2 XRS, prefer 2XRS
Details on Acronym: An Cl
An Cl	(Anonymous Cluster)= (An) (Not yet in Simbad)
Write:	<<An Cl N>>
N:	4
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Note:	Some new possible very red and faint star clusters: Proc. of the "Star Cluster Symposium", Budapest, edit. B.A. Balazz, p. 39, Pfleiderer+ 1978. An Cl 1 = C 0104+653. An Cl 2 = C 1755-050. An Cl 3 = C 2306+606. An Cl 4 = C 2348+620 (Lynga 1983 private communication)
Auth.:	PFLEIDERER J.+
Details on Acronym: [AN2004]
[AN2004]	(Ali+Noriega-Crespo, 2004)
Write:	<<[AN2004] NN>>
N:	34
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	ISOCAM data from the ISO archive of the LDN 1641N outflow region.
in source:	Orion Nebula:LDN 1641N = LDN 1641N
Ref:	=2004ApJ...613..374A
by	ALI B. , NORIEGA-CRESPO A.
	Astrophys. J., 613, 374-380 (2004)
	A mid-infrared survey of L1641N with ISOCAM.
o	Fig.2, Table 2: <[AN2004] NN> (Nos 1-34).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: And
And	(Andromeda)
Write:	<<And R>>
N:	33
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	(Nos I-XXXIII), dwarf galaxies companions of M 31. And V and And VI were discovered in 1998 by Armandroff. And X was discovered by Zucker in 2006.
Ref:	=1972ApJ...171L..31V
by	VAN DEN BERGH S.
	Astrophys. J., 171, 31-33 (1972)
	Search for faint companions to M 31.
o	<And R> (Nos I-IV).
Ref:	=1998AJ....116.2287A
by	ARMANDROFF T.E. , DAVIES J.E., JACOBY G.H.
	Astron. J., 116, 2287-2296 (1998)
	A survey for low surface brightness galaxies around M 31. I. The newly discovered dwarf Andromeda V.
o	<And R> (No. V) added.
Ref:	=1999A&A...341..355K
by	KARACHENTSEV I.D. , KARACHENTSEVA V.E.
	Astron. Astrophys., 341, 355-356 (1999)
	New probable companions to M31 found on the POSS-II.
o	Names 'Cassiopeaia dwarf' and 'Pegasus dwarf' used by authors are not used in SIMBAD. There is another 'NAME PEGASUS DWARF' used in SIMBAD, which is not 'And VI'.
o	Text: <And R> (No. VI) added. Table 1: <[KK99] FFF.N> N=4.
Ref:	=1999ApJ...511L.101G
by	GREBEL E.K. , GUHATHAKURTA P.
	Astrophys. J., 511, 101-105 (1999)
	Properties of two new M31 dwarf spheroidal companions from Keck imaging.
o	<And R> (No. VII) added.
Ref:	=2003ApJ...596L.183M
by	MORRISON H.L. , HARDING P., HURLEY-KELLER D., JACOBY G.
	Astrophys. J., 596, 183-186 (2003)
	Andromeda VIII: a new tidally distorted satellite of M31.
o	<And R> (No. VIII) added.
Ref:	=2004ApJ...612L.121Z
by	ZUCKER D.B. , KNIAZEV A.Y., BELL E.F., MARTINEZ-DELGADO D., GREBEL E.K., RIX H.-W., ROCKOSI C.M., HOLTZMAN J.A., WALTERBOS R.A.M., ANNIS J., YORK D.G., IVEZIC Z., BRINKMANN J., BREWINGTON H., HARVANEK M., HENNESSY G., KLEINMAN S.J., KRZESINSKI J., LONG D., NEWMAN P.R., NITTA A., SNEDDEN S.A.
	Astrophys. J., 612, 121-124 (2004)
	Andromeda IX: a new dwarf spheroidal satellite of M31.
o	<And R> (No. IX) added.
Ref:	=2006MNRAS.371.1983M
by	MARTIN N.F. , IBATA R.A., IRWIN M.J., CHAPMAN S., LEWIS G.F., FERGUSON A.M.N., TANVIR N., McCONNACHIE A.W.
	Mon. Not. R. Astron. Soc., 371, 1983-1991 (2006)
	Discovery and analysis of three faint dwarf galaxies and a globular cluster in the outer halo of the Andromeda galaxy.
o	Table 1: <And R> (Nos XI to XIII) added. Table 1: <[MII2006] GC> N=1.
Ref:	=2007ApJ...659L..21Z
by	ZUCKER D.B. , KNIAZEV A.Y., MARTINEZ-DELGADO D., BELL E.F., RIX H.-W., GREBEL E.K., HOLTZMAN J.A., WALTERBOS R.A.M., ROCKOSI C.M., YORK D.G., BARENTINE J.C., BREWINGTON H., BRINKMANN J., HARVANEK M., KLEINMAN S.J., KRZESINSKI J., LONG D., NEILSEN E.H.Jr, NITTA A., SNEDDEN S.A.
	Astrophys. J., 659L, 21-24 (2007)
	Andromeda X, a new dwarf spheroidal satellite of M31: photometry.
o	<And R> (No. X) added.
Ref:	=2007ApJ...668L.123M
by	MARTIN N.F. , IBATA R.A., IRWIN M.
	Astrophys. J., 668L, 123-126 (2007)
	Galactic halo stellar structures in the Triangulum-Andromeda region.
o	Fig.1: <And R> (Nos XV, XVI) added.
Ref:	=2007ApJ...670L...9M
by	MAJEWSKI S.R. , BEATON R.L., PATTERSON R.J., KALIRAI J.S., GEHA M.C., MUNOZ R.R., SEIGAR M.S., GUHATHAKURTA P., GILBERT K.M., RICH R.M., BULLOCK J.S., REITZEL D.B.
	Astrophys. J., 670L, 9-12 (2007)
	Discovery of Andromeda XIV: a dwarf spheroidal dynamical rogue in the Local Group?
o	<And R> (No. XIV) added.
Ref:	=2008ApJ...676L..17I
by	IRWIN M.J. , FERGUSON A.M.N., HUXOR A.P., TANVIR N.R., IBATA R.A., LEWIS G.F.
	Astrophys. J., 676L, 17-20 (2008)
	Andromeda XVII: a new low-luminosity satellite of M31.
o	<And R> (No. XVII) added.
Ref:	=2008ApJ...688.1009M
by	McCONNACHIE A.W. , HUXOR A., MARTIN N.F., IRWIN M.J., CHAPMAN S.C., FAHLMAN G., FERGUSON A.M.N., IBATA R.A., LEWIS G.F., RICHER H., TANVIR N.R.
	Astrophys. J., 688, 1009-1020 (2008)
	A trio of new local group galaxies with extreme properties.
o	<And R> (Nos XVIII-XX) added.
Ref:	=2009ApJ...705..758M
by	MARTIN N.F. , McCONNACHIE A.W., IRWIN M., WIDROW L.M., FERGUSON A.M.N., IBATA R.A., DUBINSKI J., BABUL A., CHAPMAN S., FARDAL M., LEWIS G.F., NAVARRO J., RICH R.M.
	Astrophys. J., 705, 758-765 (2009)
	PAndAS' CUBS: discovery of two new dwarf galaxies in the surroundings of the Andromeda and Triangulum galaxies.
o	<And R> (Nos XXI-XXII) added. <Psc R> (Nos I-V).
Ref:	=2011ApJ...732...76R
by	RICHARDSON J.C. , IRWIN M.J., McCONNACHIE A.W., MARTIN N.F., DOTTER A.L., FERGUSON A.M.N., IBATA R.A., CHAPMAN S.C., LEWIS G.F., TANVIR N.R., RICH R.M.
	Astrophys. J., 732, 76 (2011)
	PAndAS' progeny: extending the M31 dwarf galaxy cabal.
o	<And R> (Nos XXIII-XXVII) added.
Ref:	=2011ApJ...742L..14S
by	SLATER C.T. , BELL E.F., MARTIN N.F.
	Astrophys. J., 742L, 14 (2011)
	Andromeda XXVIII: a dwarf galaxy more than 350 kpc from Andromeda.
o	<And R> (No. XXVIII) added.
Ref:	=2011ApJ...742L..15B
by	BELL E.F. , SLATER C.T., MARTIN N.F.
	Astrophys. J., 742L, 15 (2011)
	Andromeda XXIX: a new dwarf spheroidal galaxy 200 kpc from Andromeda.
o	<And R> (No. XXIX) added.
Ref:	=2013ApJ...772...15M
by	MARTIN N.F. , SLATER C.T., SCHLAFLY E.F., MORGANSON E., RIX H.-W., BELL E.F., LAEVENS B.P.M., BERNARD E.J., FERGUSON A.M.N., FINKBEINER D.P., BURGETT W.S., CHAMBERS K.C., HODAPP K.W., KAISER N., KUDRITZKI R.-P., MAGNIER E.A., MORGAN J.S., PRICE P.A., TONRY J.L., WAINSCOAT R.J.
	Astrophys. J., 772, 15 (2013)
	Lacerta I and Cassiopeia III. Two luminous and distant Andromeda satellite dwarf galaxies found in the 3π Pan-STARRS1 survey.
o	<And R> (Nos XXXI-XXXII) added. <NAME Lacerta I> N=1. <NAME Cassiopeia III> N=1.
Ref:	=2013ApJ...779L..10M
by	MARTIN N.F. , SCHLAFLY E.F., SLATER C.T., BERNARD E.J., RIX H.-W., BELL E.F., FERGUSON A.M.N., FINKBEINER D.P., LAEVENS B.P.M., BURGETT W.S., CHAMBERS K.C., DRAPER P.W., HODAPP K.W., KAISER N., KUDRITZKI R.-P., MAGNIER E.A., METCALFE N., MORGAN J.S., PRICE P.A., TONRY J.L., WAINSCOAT R.J., WATERS C.
	Astrophys. J., 779L, 10 (2013)
	Perseus I: a distant satellite dwarf galaxy of Andromeda.
o	<And R> (No. XXXIII) added. <NAME Perseus I Dwarf Galaxy> = <NAME Per I Dwarf Galaxy>.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: And
And	(Andromeda)
Write:	<<And HHMM+DDd>>
N:	23
Object:	Blue (SIMBAD class: blue = Blue Object)
Stat:	is completely incorporated in Simbad
Ref:	=1993ApJ...411..650M
by	McCAUSLAND R.J.H. , CONLON E.S., DUFTON P.L., FITZSIMMONS A., IRWIN M.J., KEENAN F.P.
	Astrophys. J., 411, 650-654 (1993)
	A search for young stars in the halo of M 31.
o	<And HHMM+DDd> N=23
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Andrews
Andrews	(Andrews)= (A) = ADA
Write:	<<Andrews NNNNN>>
N:	16777
Object:	* (SIMBAD class: Star)
Note:	Andrews + Grossie, 1981, Atlas, Armagh Observatory, A photometric atlas of the Orion nebula.
in source:	NAME Orion Nebula
Auth.:	ANDREWS A.D.+
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [ANE99]
[ANE99]	(Arkhipova+Noskova+Esipov+, 1999) (Not yet in Simbad)
Write:	<<[ANE99] a>>
N:	4
Object:	* (SIMBAD class: Star)
Note:	N=4 comparison stars among (Nos a-e) in the field of V4334 Sgr. Fig.1: finding chart of V4334 Sgr with the comparison stars.
Ref:	=1999AstL...25..615A
by	ARKHIPOVA V.P. , NOSKOVA R.I., ESIPOV V.F., SOKOL G.V.
	Astron. Lett., 25, 615-623 (1999)
	Sakurai's object (V4334 Sgr) in 1998: the R CrB phase has set in.
o	1999PAZh...25..711A
o	Table 1: <[ANE99] a> (Nos a, c-e).
=E=	Catalogue in electronic form as II/229
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ANEPD-CXO
ANEPD-CXO	(AKARI North Ecliptic Pole Deep Field Chandra X-ray Observatory) (Not yet in Simbad)
Write:	<<ANEPD-CXO NNN>> <<ANEPD-CXO sNNN>>
N:	457+626
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of N=457+626 X-ray sources (in the main and low likelihood source, or "supplementary", catalog respectively) in the AKARI North Ecliptic Pole Deep Field.
Ref:	=2015MNRAS.446..911K
by	KRUMPE M. , MIYAJI T., BRUNNER H., HANAMI H., ISHIGAKI T., TAKAGI T., MARKOWITZ A.G., GOTO T., MALKAN M.A., MATSUHARA H., PEARSON C., UEDA Y., WADA T.
	Mon. Not. R. Astron. Soc., 446, 911-931 (2015)
	Chandra survey in the AKARI North Ecliptic Pole Deep Field - I. X-ray data, point-like source catalogue, sensitivity maps, and number counts.
o	maincat: <ANEPD-CXONNN> (Nos CXO001-CXO457). lowpscat: <ANEPD-CXOsNNN> (Nos CXOs001-CXOs626).
=E=	Catalogue in electronic form as <J/MNRAS/446/911/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ANGST
ANGST	(ACS Nearby Galaxy Survey Treasury)
Write:	<<ANGST CNN>> <<ANGST OVN>>
N:	11+2
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations of the outer disk of M81, allowing to distinguish between fundamental mode (CNN) and first overtone (OVN) cepheids.
in source:	M 81
Ref:	=2009AJ....137.4707M
by	McCOMMAS L.P. , YOACHIM P., WILLIAMS B.F., DALCANTON J.J., DAVIS M.R., DOLPHIN A.E.
	Astron. J., 137, 4707-4715 (2009)
	The ACS Nearby Galaxy Survey Treasury. III. Cepheids in the outer disk of M81.
o	Table 4: <ANGST CNN> (Nos C1-C11). Table 5: <ANGST OVN> (Nos OV1, OV2).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ANK2017]
[ANK2017]	(Ando+Nakanishi+Kohno+, 2017)
Write:	<<[ANK2017] Clump N>>
N:	8
Object:	Clump (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 7 observations of N=8 dusty star-forming clumps in the central region of NGC 253.
in source:	NGC 253
Ref:	=2017ApJ...849...81A
by	ANDO R. , NAKANISHI K., KOHNO K., IZUMI T., MARTIN S., HARADA N., TAKANO S., KUNO N., NAKAI N., SUGAI H., SORAI K., TOSAKI T., MATSUBAYASHI K., NAKAJIMA T., NISHIMURA Y., TAMURA Y.
	Astrophys. J., 849, 81-81 (2017)
	Diverse nuclear star-forming activities in the heart of NGC 253 resolved with 10-pc-scale ALMA images.
o	Figs 1-2, Tables 1-2: <[ANK2017] Clump N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ANL97]
[ANL97]	(Armus+Neugebauer+Lehnert+, 1997)
Write:	<<[ANL97] 4C +09.17 A>>
N:	4
Object:	(Near IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	NIR images of 4C +09.17 reveal 3 companions: (Nos B-D), No. A = 4C +09.17.
Ref:	=1997MNRAS.289..621A
by	ARMUS L. , NEUGEBAUER G., LEHNERT M.D., MATTHEWS K.
	Mon. Not. R. Astron. Soc., 289, 621-628 (1997)
	The unusual near-infrared morphology of the radio-loud quasar 4C +09.17.
o	Fig.1, Table 1: <[ANL97] 4C +09.17 A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ANM2019]
[ANM2019]	(Alonso-Santiago+Negueruela+Marco+, 2019)
Write:	<<[ANM2019] NNNN>>
N:	2153
Object:	* (SIMBAD class: Star)
Note:	INT WFC photometry and AAT AAOMEGA, La Palma 2.5-m INT IDS, WHT ISIS, WHT WYFFOS, ESO/MPG 2.2-m telescope FEROS spectroscopy of N=2153 stars in the field of the open cluster NGC 2345.
in source:	NGC 2345
Ref:	=2019A&A...631A.124A
by	ALONSO-SANTIAGO J. , NEGUERUELA I., MARCO A., TABERNERO H.M., GONZALEZ-FERNANDEZ C., CASTRO N.
	Astron. Astrophys., 631A, 124-124 (2019)
	A comprehensive study of NGC 2345, a young open cluster with a low metallicity.
o	Table A.1: <[ANM2019] NNNN> (Nos 1-2153).
=E=	Catalogue in electronic form as <J/A+A/631/A124/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ANM98]
[ANM98]	(Adami+Nichol+Mazure+, 1998)
Write:	<<[ANM98] +x.xx+y.yy>>
N:	32
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
in source:	Coma Cluster = ACO 1656
Ref:	=1998A&A...334..765A
by	ADAMI C. , NICHOL R.C., MAZURE A., DURRET F., HOLDEN B., LOBO C.
	Astron. Astrophys., 334, 765-769 (1998)
	Deep probing of the Coma cluster.
o	Table 1: <[ANM98] +X.xx+Y.yy> N=32.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ann. Bok
Ann. Bok	(Anonymous, Discoverer's name)
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Ref:	=1977PASP...89..554P
by	PHILIP A.G.D. , DEMARQUE P., SWEIGART A.V., CIARDULLO R.B.
	Publ. Astron. Soc. Pac., 89, 554-556 (1977)
	A comparison of observations with main-sequence evolutionary models.
o	<NAME Bok OCl>
*****	Avoid the usage of Ann. Bok, prefer Bok
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Annizam
Annizam	(Annizam)
Write:	<<Annizam NNNNNNN>>
N:	181
Object:	* (SIMBAD class: Star)
Note:	Stars surrounding the star system Alnilam. Use of archival Tycho-2, DENIS, and 2MASS data. See also Mantaqah, EOri.
Ref:	=2008A&A...485..931C
by	CABALLERO J.A. , SOLANO E.
	Astron. Astrophys., 485, 931-949 (2008)
	Young stars and brown dwarfs surrounding Alnilam (ε Orionis) and Mintaka (δ Orionis).
o	Notes to table A.6 p.943 TYC 4767-2257-1 is a probable misprint for TYC 4766-757-1
o	Tables a9, a11: <EOri N-NNNN> N=9. Tables a9, a16: <Annizam NNNNNN> N=181. Tables a10, a17: <Mantaqah NNNNNNN> N=103.
=E=	Catalogue in electronic form as <J/A+A/485/931/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Anon
Anon	(Not yet in Simbad)
*****	Avoid the usage of Anon, prefer [I68]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Anon
Anon	(Anonymous)= (A) = (Anonym) = Anonymous
Write:	<<Anon HHMM+DDA>> <<Anon HHMM+DDd>> <<Anon HHMM+DD.d>> <<Anon HHMM+DDMMW>> <<Anon HHMM.m+DDMMW>> <<Anon HHMMSS+DDMMSS>> <<Anon HHMMSS.s+DDMMSS>>
Object:	G (SIMBAD class: Galaxy)
Note:	From the RC1, RC2 VII/112, RC3 VII/155 catalogues of De Vaucouleurs
=E=	Catalogue in electronic form as VII/112
=E=	Catalogue in electronic form as VII/155
Details on Acronym: Anon
Anon	(Anonymous)
Write:	<<Anon JHHMMSS+DDMM>> <<Anon AHHMMSS+DDMM>> (not recognised by Simbad, but found in literature)
N:	2443
Object:	G (SIMBAD class: Galaxy)
Note:	Anonymous host galaxies of SN in the new Asiago Supernova Catalogue.
Ref:	=2008yCat.2283....0B
by	BARBON R. , BUONDI V., CAPPELLARO E., TURATTO M.
	yCat, 2283, 0 (2008)
	Asiago Supernova Catalogue (Version 2008-Mar).
o	Catalogue: <Anon JHHMMSS+DDMM> N=2443.
=E=	Catalogue in electronic form as II/283
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Anon
Anon	(Anonymous)
*****	Avoid the usage of Anon, prefer [B80]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Anon
Anon	(Anonymous)
*****	Avoid the usage of Anon, prefer [H60b]
Details on Acronym: Anon
Anon	(Anonymous)
*****	Avoid the usage of Anon, prefer [KSS73]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Anon
Anon	(Anonymous)
*****	Avoid the usage of Anon, prefer [SD76]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Anonym
Anonym	(Anonymous)
*****	Avoid the usage of Anonym, prefer Anon
Details on Acronym: Anonymous
Anonymous	(Anonymous)
====>	Equivalent to: Anon
Details on Acronym: ANS
ANS	(Astron. Netherland satellite) (Not yet in Simbad)
Write:	<<ANS HHMM+DD>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Details on Acronym: Antalova
Antalova	(Antalova)= (Av)
Write:	<<Antalova OB-NNN>> <<Antalova IS-NNN>> <<Antalova Cloud A>>
N:	250+101+3
Object:	* + Em. region (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Catalogue: N=250 OB stars and 101 'IS' (Interesting stars). Text: N=3 region or group of objects, called 'Cloud A' to 'Cloud C'.
Ref:	=1970BAICz..21..331A
by	ANTALOVA A.
	Bull. Astron. Inst. Czech., 21, 331-344 (1970)
	UBV photographic photometry of stars in the region AR 1950 17.03-17.41, Dec 1950 28.8-33.4. I. The catalogue and identification maps of 25 0 OB and 101 photometrically interesting stars.
o	Catalogue: <Antalova OB-NNN> (Nos OB-1 to OB-250), <Antalova IS-NNN> (Nos IS-1 to IS-101). Text: <Antalova Cloud A> (Nos A-C). Map 7: <CL Antalova N> (Nos 1-3). Map: <Cl* NGC 6374 Ant A> (Nos A-F).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Antalova
Antalova	(Antalova)= (Av)
Write:	<<Cl Antalova N>>
N:	3
Object:	OCl (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Map 7: Cl Antalova 1 = C 1725-315, Em. region behind Gum 68 Cl Antalova 2 = C 1726-324, OCl Cl Antalova 3 = Em. region behind Gum 67
Ref:	=1970BAICz..21..331A
by	ANTALOVA A.
	Bull. Astron. Inst. Czech., 21, 331-344 (1970)
	UBV photographic photometry of stars in the region AR 1950 17.03-17.41, Dec 1950 28.8-33.4. I. The catalogue and identification maps of 25 0 OB and 101 photometrically interesting stars.
o	Catalogue: <Antalova OB-NNN> (Nos OB-1 to OB-250), <Antalova IS-NNN> (Nos IS-1 to IS-101). Text: <Antalova Cloud A> (Nos A-C). Map 7: <CL Antalova N> (Nos 1-3). Map: <Cl* NGC 6374 Ant A> (Nos A-F).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Antennae
Antennae	(the Antennae)
*****	Avoid the usage of Antennae, prefer [ZFR2002]
Origin	of the Acronym: L (2004ApJ...614L.117M)
Details on Acronym: Antipin
Antipin	(Antipin)
Write:	<<Antipin VNN>>
N:	81
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	called Var NN by the author Antipin S.V. (Nos V52-V60, V72) missing.
Ref:	=1994IBVS.4125....1A
by	ANTIPIN S.V.
	IAU Inform. Bull. Var. Stars, 4125, 1-4 (1994)
	Ten new variable stars in Hercules and Corona Borealis.
o	<Antipin VNN> (Nos V1-V10)
Ref:	=1996IBVS.4342....1A
by	ANTIPIN S.V.
	IAU Inform. Bull. Var. Stars, 4342, 1-4 (1996)
	New variable stars in the η Herculis field.
o	Fig.1: comparison stars 'a' not in SIMBAD.
o	<Antipin VNN> (Nos V11-V18)
Ref:	=1996IBVS.4343....1A
by	ANTIPIN S.V.
	IAU Inform. Bull. Var. Stars, 4343, 1-4 (1996)
	New variable stars in the eps Coronae Borealis field.
o	Fig.1: comparison stars 'a' not in SIMBAD.
o	<Antipin VNN> (Nos V19-V24)
Ref:	=1996IBVS.4344....1A
by	ANTIPIN S.V.
	IAU Inform. Bull. Var. Stars, 4344, 1-4 (1996)
	New variable stars in the 66 Ophiuchi field.
o	Fig.1: comparison stars 'a' not in SIMBAD.
o	<Antipin VNN> (Nos V25-V33)
Ref:	=1996IBVS.4345....1A
by	ANTIPIN S.V.
	IAU Inform. Bull. Var. Stars, 4345, 1-4 (1996)
	Nine new variables in the 66 Ophiuchi field.
o	Fig.1: comparison stars 'a' not in SIMBAD.
o	<Antipin VNN> (Nos V34-V42)
Ref:	=1996IBVS.4360....1A
by	ANTIPIN S.V.
	IAU Inform. Bull. Var. Stars, 4360, 1-4 (1996)
	Nine new variables in the η Herculis field.
o	Fig.1: comparison stars 'a' not in SIMBAD.
o	<Antipin VNN> (Nos V43-V51)
Ref:	=1998IBVS.4578....1A
by	ANTIPIN S.V.
	IAU Inform. Bull. Var. Stars, 4578, 1-4 (1998)
	Var 61 Her, Var 62 And, KUV 23012+1702: new dwarf novae on Moscow plates.
o	Fig.1: comparison stars 'a' not in SIMBAD.
o	<Antipin VNN> (Nos V61-V62)
Ref:	=1999IBVS.4673....1A
by	ANTIPIN S.V.
	IAU Inform. Bull. Var. Stars, 4673, 1-4 (1999)
	New dwarf novae on Moscow plates II.
o	Fig.1: comparison stars 'a' not in SIMBAD.
o	<Antipin VNN> (Nos V63-V66).
Ref:	=1999IBVS.4699....1A
by	ANTIPIN S.V.
	IAU Inform. Bull. Var. Stars, 4699, 1-4 (1999)
	New cepheids in Aquila.
o	Fig.1: comparison stars 'a' not in SIMBAD.
o	<Antipin VNN> (Nos V67-V68).
Ref:	=1999IBVS.4772....1A
by	ANTIPIN S.V.
	IAU Inform. Bull. Var. Stars, 4772, 1-2 (1999)
	A new classical Cepheid in Sagitta.
o	Fig.1: comparison stars 'a' not in SIMBAD.
o	<Antipin VNN> (No. V69).
Ref:	=2000IBVS.4938....1A
by	ANTIPIN S.V.
	IAU Inform. Bull. Var. Stars, 4938, 1-None (2000)
	A new classical cepheid in Cassiopeia.
o	<Antipin VNN> (No. V70).
Ref:	=2000IBVS.4939....1A
by	ANTIPIN S.V.
	IAU Inform. Bull. Var. Stars, 4939, 1-None (2000)
	A new high amplitude short period variable star in Cassiopeia.
o	<Antipin VNN> (No. V71).
Ref:	=2002A&A...391..565A
by	ANTIPIN S.V. , PAVLENKO E.P.
	Astron. Astrophys., 391, 565-569 (2002)
	Discovery and photometric study of the new in-the-gap SU UMa dwarf nova Var 73 Dra.
o	<Antipin VNN> (No. V73).
Ref:	=2002IBVS.5265....1A
by	ANTIPIN S.V.
	IAU Inform. Bull. Var. Stars, 5265, 1-None (2002)
	A new 7-day classical cepheid in Cassiopeia.
o	<Antipin VNN> (No. V74).
Ref:	=2003IBVS.5461....1A
by	ANTIPIN S.V. , KROLL P.
	IAU Inform. Bull. Var. Stars, 5461, 1-None (2003)
	Discovery of two new dwarf novae in Cepheus and Cygnus.
o	<Antipin VNN> (Nos V75, V76).
Ref:	=2004IBVS.5573....1A
by	ANTIPIN S.V.
	IAU Inform. Bull. Var. Stars, 5573, 1-None (2004)
	New dwarf novae on Moscow plates III.
o	Comparison stars are not in SIMBAD
o	<Antipin VNN> (Nos V79, V80).
Ref:	=2005IBVS.5600....1.
by	:Anonymous
	IAU Inform. Bull. Var. Stars, 5600, 1-None (2005)
	Variability Notes: Reports on new discoveries.
o	<Antipin VNN> (Nos V77, V78, V81).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ANTL
ANTL	(Antlia Cluster)= ([SCF2012])
Write:	<<ANTL JHHMMSS+DDMMSS>> <<ANTL JHHMMSS+DDMMSS.s>> <<ANTL JHHMMSS.s+DDMMSS.s>>
N:	5+16+7+18+11+147
Object:	Poss. G + G (SIMBAD class: Galaxy_Candidate = Galaxy Candidate)
Note:	CTIO Blanco 4m telescope MOSAIC II, VLT VIMOS, Gemini GMOS observations of galaxies in the central region of the Antlia cluster. See also [FS90].
in source:	NAME Antlia Cluster
Ref:	=2012MNRAS.419.2472S
by	SMITH CASTELLI A.V. , CELLONE S.A., FAIFER F.R., BASSINO L.P., RICHTLER T., ROMERO G.A., CALDERON J.P., CASO J.P.
	Mon. Not. R. Astron. Soc., 419, 2472-2488 (2012)
	Galaxy populations in the Antlia cluster - III. Properties of faint early-type galaxies.
o	Table B1: <ANTL JHHMMSS+DDMMSS.s> N=5. Table B2: <ANTL JHHMMSS+DDMMSS> N=16.
Ref:	=2015MNRAS.451..791C
by	CALDERON J.P. , BASSINO L.P., CELLONE S.A., RICHTLER T., CASO J.P., GOMEZ M.
	Mon. Not. R. Astron. Soc., 451, 791-803 (2015)
	Early-type galaxies in the Antlia Cluster: a deep look into scaling relations.
o	Table 3: <ANTL JHHMMSS.s+DDMMSS.s> N=7.
Ref:	=2015A&A...584A.125C
by	CASO J.P. , RICHTLER T.
	Astron. Astrophys., 584A, 125-125 (2015)
	Deconstructing the Antlia cluster core.
o	Table A.1: <ANTL JHHMMSS+DDMMSS> N=18 added. Table A.2: <ANTL JHHMMSS+DDMMSS> N=11 added.
Ref:	=2020MNRAS.497.1791C
by	CALDERON J.P. , BASSINO L.P., CELLONE S.A., GOMEZ M., CASO J.P.
	Mon. Not. R. Astron. Soc., 497, 1791-1806 (2020)
	Early-type galaxies in the Antlia cluster: global properties.
o	Table 3: <ANTL JHHMMSS.s+DDMMSS.s> N=147 added.
=E=	Catalogue in electronic form as <J/MNRAS/497/1791/>
Origin	of the Acronym: A = Assigned by the author(s)
History	of this Acronym: replaces [SCF2012]
Details on Acronym: [ANW2017]
[ANW2017]	(Auchettl+Ng+Wong+, 2017)
Write:	<<[ANW2017] NN>>
N:	25
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton MOS and PN observations of N=25 sources in the field of the molecular cloud SNR G346.6-0.2.
in source:	SNR G346.6-00.2
Ref:	=2017ApJ...847..121A
by	AUCHETTL K. , NG C.-Y., WONG B.T.T., LOPEZ L., SLANE P.
	Astrophys. J., 847, 121-121 (2017)
	An XMM-Newton study of the mixed-morphology supernova remnant G346.6-0.2.
o	Tables 3-4: <[ANW2017] NN> (Nos 1-25).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AO
AO	(Arecibo obs., Occultation)
Write:	<<AO HHMM+DDA>>
N:	35
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Identif. charts.
Ref:	=1967ApJ...148..669H
by	HAZARD C. , GULKIS S., BRAY A.D.
	Astrophys. J., 148, 669-688 (1967)
	Lunar occultation studies of 5 weak radio sources of small angular size.
o	Table 1: <AO HHMM+DDA> N=6
Ref:	=1968ApJ...154..413H
by	HAZARD C. , GULKIS S., SUTTON J.
	Astrophys. J., 154, 413-422 (1968)
	Occultation studies of weak radio sources: list 2.
o	Table 1: <AO HHMM+DDA> N=12
Ref:	=1969ApJ...157.1047G
by	GULKIS S. , SUTTON J., HAZARD C.
	Astrophys. J., 157, 1047-1053 (1969)
	Arecibo occultation studies: list 3.
o	Table 1: <AO HHMM+DDA> N=11
Ref:	=1970ApJ...160...17L
by	LANG K.R. , SUTTON J., HAZARD C., GULKIS S.
	Astrophys. J., 160, 17-23 (1970)
	Additional occultation studies of weak radio sources at Arecibo Observatory: list 4.
o	Table 1: <AO HHMM+DDA> N=10
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AO
AO	(Allegheny Obs.)
*****	Avoid the usage of AO, prefer Gat
Details on Acronym: AO
AO	(Adaptative Optics)
*****	Avoid the usage of AO, prefer [SCB99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AO84]
[AO84]	(Agekian+Orlov, 1984) (Not yet in Simbad)
Write:	<<[AO84] R NN>>
N:	155
Object:	* in Cl* (SIMBAD class: Star)
Note:	Format 'R NN' for * in each cluster (I to IX)
Ref:	=1984AZh....61...60A
by	AGEKIAN T.A. , ORLOV V.V.
	Astron. Zh., 61, 60-None (1984)
	The membership of stars of solar neighbourhood in moving clusters.
o	<[AO84] R> N=9, <[AO84] R NN> N=155
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AO84]
[AO84]	(Agekian+Orlov, 1984)
Write:	<<[AO84] R>>
N:	9
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Format 'R' (roman numeral) for possible clusters, I to IX, N=9
Ref:	=1984AZh....61...60A
by	AGEKIAN T.A. , ORLOV V.V.
	Astron. Zh., 61, 60-None (1984)
	The membership of stars of solar neighbourhood in moving clusters.
o	<[AO84] R> N=9, <[AO84] R NN> N=155
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AO95]
[AO95]	(Andersen+Owen, 1995)
Write:	<<[AO95] HHMM+DDdA>> <<[AO95] HHMM+DDMM>> <<[AO95] HHMM.m+DDMM>>
N:	73
Object:	G (SIMBAD class: Galaxy)
Ref:	=1995AJ....109.1582A
by	ANDERSEN V. , OWEN F.N.
	Astron. J., 109, 1582-1591 (1995)
	The far-infrared-radio relation in cluster spiral galaxies.
o	1120+436 misprint for [AO95] 1120+346
o	Tables 1-5: <[AO95] HHMM+DDdA>, <[AO95] HHMM+DDMM>, <[AO95] HHMM.m+DDMM> N=73
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AOB2017]
[AOB2017]	(Asvathaman+Omand+Barton+, 2017)
Write:	<<[AOB2017] NN>>
N:	8
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	N=8 gamma sources not associated with 3FGL sources, detected with the FermiFAST algorithm in Fermi data and located outside the Galactic plane (\|b\|>10°).
Ref:	=2017MNRAS.466.2378A
by	ASVATHAMAN A. , OMAND C., BARTON A., HEYL J.S.
	Mon. Not. R. Astron. Soc., 466, 2378-2389 (2017)
	A fast algorithm for finding point sources in the Fermi data stream: FermiFAST.
o	Table 4: <[AOB2017] NN> N=8 among (Nos 5-43).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AOC
AOC	(Alves de Oliveira+Casali)
Write:	<<AOC JHHMMSS.ss+DDMMSS.s>>
N:	137+39
Object:	[NIR] + Y? + YO (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	Deepest near-IR variability survey of YSOs targeting rho Ophiuchi, using the WFCAM UKIRT. Variability characteristics are compared to existing models of YSOs in order to relate them to physical processes, and then used to select new candidate members of this star forming region.
in source:	NAME rho Oph Cloud
Ref:	=2008A&A...485..155A
by	ALVES DE OLIVEIRA C. , CASALI M.
	Astron. Astrophys., 485, 155-166 (2008)
	Deep near-IR variability survey of pre-main-sequence stars in ρ Ophiuchi.
o	Tables 4, a1: <AOC JHHMMSS.ss+DDMMSS.s> N=137+39.
=E=	Catalogue in electronic form as J/A+A/485/155
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: AOH
AOH	(Aaronson+Olszewski+Hodge)
Write:	<<AOH N>>
N:	6
Object:	red * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	1st ref., Table 1: red stars in Leo II, (Nos 1-5) 2nd ref., table 17: No. 6 is added
in source:	UGC 6253 = Leo II
Ref:	=1983ApJ...267..271A
by	AARONSON M. , OLSZEWSKI E.W., HODGE P.W.
	Astrophys. J., 267, 271-279 (1983)
	Carbon stars and the seven dwarfs.
o	<AOH N> N=5
Ref:	=1991AJ....101.1377E
by	EGGEN O.J. , IBEN I.Jr
	Astron. J., 101, 1377-1407 (1991)
	First giant branch and asymptotic giant branch stars in nearby aggregates.
o	Table 17, in Leo I: B81 = ALW 3, B86 = ALW 2, B108 = ALW 5, C55 = ALW 7
o	Table 17, in Leo II: <AOH N> No. 6 added
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [AOI2004]
[AOI2004]	(Ando+Ohta+Iwata+, 2004)
Write:	<<[AOI2004] N>>
N:	8
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Subaru spectroscopic observations of a sample of Lyman Break Galaxies at z about 5 in a region centered on the HDFN.
in source:	NAME HDFN
Ref:	=2004ApJ...610..635A
by	ANDO M. , OHTA K., IWATA I., WATANABE C., TAMURA N., AKIYAMA M., AOKI K.
	Astrophys. J., 610, 635-641 (2004)
	Lyman break galaxies at z~5: rest-frame ultraviolet spectra.
o	Table 1: <[AOI2004] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AOP94]
[AOP94]	(Anosova+Orlov+Pavlova, 1994)
Write:	<<[AOP94] NN>>
N:	11
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 9: N=11, satellites of alf Cen system
Ref:	=1994A&A...292..115A
by	ANOSOVA J. , ORLOV V.V., PAVLOVA N.A.
	Astron. Astrophys., 292, 115-118 (1994)
	Dynamics of nearby multiple stars. The α Centauri system.
o	Table 9: <[AOP94] NN> N=11
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AOY2000]
[AOY2000]	(Akiyama+Ohta+Yamada+, 2000)
Write:	<<[AOY2000] AX JHHMMSS+DDMM A>> <<[AOY2000] LSSN-NN>>
N:	48+25
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=48 candidate optical counterparts of 34 AX sources with increasing distance (A,B,C). Z is an additional object which was observed spectroscopically. Finding charts in Fig.1. N=25 ROSAT HRI observations of X-ray sources in ASCA LSS (Large Sky Survey) fields 1 and 2.
Ref:	=2000ApJ...532..700A
by	AKIYAMA M. , OHTA K., YAMADA T., KASHIKAWA N., YAGI M., KAWASAKI W., SAKANO M., TSURU T., UEDA Y., TAKAHASHI T., LEHMANN I., HASINGER G., VOGES W.
	Astrophys. J., 532, 700-727 (2000)
	Optical identification of the ASCA large sky survey.
o	Several 1RXS J... do not exist in the RASS catalogue. Some are replaced by existing 1RXS, the others are renamed RX J...
o	Table 2: <[AOY2000] AX JHHMMSS+DDMM A> N=48. Table 6: <[AOY2000] LSS1-NN> (Nos 1-01 to 1-11), <[AOY2000] LSS2-NN> (Nos 2-01 to 2-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AOY98]
[AOY98]	(Akiyama+Ohta+Yamada+, 1998)
Write:	<<[AOY98] Galaxy A>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Optical Identif. of AX J1315.0+3141.
Ref:	=1998ApJ...500..173A
by	AKIYAMA M. , OHTA K., TORU Y., ERACLEOUS M., HALPERN J.P., KASHIKAWA N., YAGI M., KAWASAKI W., SAKANO M., TSURU T., UEDA Y., TAKAHASHI T.
	Astrophys. J., 500, 173-180 (1998)
	Optical identification of the hardest X-ray source in the ASCA large-sky survey.
o	Tables 1, 2: <[AOY98] Galaxy A> (Nos A-C)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AOZ2010]
[AOZ2010]	(Adamo+Ostlin+Zackrisson+, 2010) (Not yet in Simbad)
Write:	<<[AOZ2010] NNN>>
N:	4
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST WFPC2 and NICMOS observations of N=4 star clusters in Haro 11. Use of archival HST ACS images.
in source:	[H56] 11
Ref:	=2010MNRAS.407..870A
by	ADAMO A. , OSTLIN G., ZACKRISSON E., HAYES M., CUMMING R.J., MICHEVA G.
	Mon. Not. R. Astron. Soc., 407, 870-890 (2010)
	Super star clusters in Haro 11: properties of a very young starburst and evidence for a near-infrared flux excess.
o	Fig. 4, Table B1: <[AOZ2010] NNN> (Nos 6, 43, 87, 113).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AOZ2011]
[AOZ2011]	(Adamo+Ostlin+Zackrisson+, 2011) (Not yet in Simbad)
Write:	<<[AOZ2011] NNN>>
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST observations of star clusters in the galaxy ESO 185-13.
in source:	ESO 185-13
Ref:	=2011MNRAS.414.1793A
by	ADAMO A. , OSTLIN G., ZACKRISSON E., HAYES M.
	Mon. Not. R. Astron. Soc., 414, 1793-1812 (2011)
	The massive star clusters in the dwarf merger ESO 185-IG13: is the red excess ubiquitous in starbursts?
o	Table 2: <[AOZ2011] NNN> N=14 among (Nos 56-344).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AP
AP	(APOGEE)= (APOGEE)
Write:	<<AP JHHMMSSss+DDMMSSs>>
N:	6562+8833
Object:	* (SIMBAD class: Star)
Note:	The APO Galactic Evolution Experiment (APOGEE) is a large-scale, stellar spectroscopic survey conducted in the near-infrared (H-band). It consists of two generations APOGEE-1 (SDSS-III) and APOGEE-2 (SDSS-IV). APOGEE-2 is subdivided in APOGEE-2N and APOGEE-2S, which are being carried out from the Northern and Southern hemispheres, respectively, using the Apache Point Observatory (APO) 2.5 m Sloan Foundation telescope and the Las Campanas Observatory (LCO) 2.5 m du Pont telescope. DR16 is the first data release that includes data from the southern instrument/telescope. For more information, visit: https://www.sdss.org/surveys/apogee/ https://www.sdss.org/surveys/apogee-2/
Notes:	In SIMBAD, the acronym is applied to the whole catalog, not taking into account the first two characters (2M for 2MASS or AP for APOGEE identifiers respectively).
Ref:	=2020AJ....160..120J
by	JONSSON H. , HOLTZMAN J.A., ALLENDE PRIETO C., CUNHA K., GARCIA-HERNANDEZ D.A., HASSELQUIST S., MASSERON T., OSORIO Y., SHETRONE M., SMITH V., STRINGFELLOW G.S., BIZYAEV D., EDVARDSSON B., MAJEWSKI S.R., MESZAROS S., SOUTO D., ZAMORA O., BEATON R.L., BOVY J., DONOR J., PINSONNEAULT M.H., POOVELIL V.J., SOBECK J.
	Astron. J., 160, 120-120 (2020)
	APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South.
o	All the sources with a 2MASS identifier and SaFlag = 0 (Flag for star condition) - about 365,700 unique objects - have been ingested in SIMBAD.
o	<AP JHHMMSSss+DDMMSSs>.
Ref:	=2022ApJS..259...35A
by	ABDURRO'UF , ACCETTA K., AERTS C., SILVA AGUIRRE V., AHUMADA R., AJGAONKAR N., AK N.F., ALAM S., ALLENDE PRIETO C., ALMEIDA A., ANDERS F., ANDERSON S.F., ANDREWS B.H., ANGUIANO B., AQUINO-ORTIZ E., ARAGON-SALAMANCA A., ARGUDO-FERNANDEZ M., ATA M., AUBERT M., AVILA-REESE V., BADENES C., BARBA R.H., BARGER K., BARRERA-BALLESTEROS J.K., BEATON R.L., BEERS T.C., BELFIORE F., BENDER C.F., BERNARDI M., BERSHADY M.A., BEUTLER F., BIDIN C.M., BIRD J.C., BIZYAEV D., BLANC G.A., BLANTON M.R., BOARDMAN N.F., BOLTON A.S., BOQUIEN M., BORISSOVA J., BOVY J., BRANDT W.N., BROWN J., BROWNSTEIN J.R., BRUSA M., BUCHNER J., BUNDY K., BURCHETT J.N., BUREAU M., BURGASSER A., CABANG T.K., CAMPBELL S., CAPPELLARI M., CARLBERG J.K., CARNEIRO WANDERLEY F., CARRERA R., CASH J., CHEN Y.-P., CHEN W.-H., CHERINKA B., CHIAPPINI C., CHOI P.D., CHOJNOWSKI S.D., CHUNG H., CLERC N., COHEN R.E., COMERFORD J.M., COMPARAT J., DA COSTA L., COVEY K., CRANE J.D., CRUZ-GONZALEZ I., CULHANE C., CUNHA K., DAI Y.S., DAMKE G., DARLING J., DAVIDSON J.W.Jr, DAVIES R., DAWSON K., DE LEE N., DIAMOND-STANIC A.M., CANO-DIAZ M., DOMINGUEZ SANCHEZ H., DONOR J., DUCKWORTH C., DWELLY T., EISENSTEIN D.J., ELSWORTH Y.P., EMSELLEM E., ERACLEOUS M., ESCOFFIER S., FAN X., FARR E., FENG S., FERNANDEZ-TRINCADO J.G., FEUILLET D., FILIPP A., FILLINGHAM S.P., FRINCHABOY P.M., FROMENTEAU S., GALBANY L., GARCIA R.A., GARCIA-HERNANDEZ D.A., GE J., GEISLER D., GELFAND J., GERON T., GIBSON B.J., GODDY J., GODOY-RIVERA D., GRABOWSKI K., GREEN P.J., GREENER M., GRIER C.J., GRIFFITH E., GUO H., GUY J., HADJARA M., HARDING P., HASSELQUIST S., HAYES C.R., HEARTY F., HERNANDEZ J., HILL L., HOGG D.W., HOLTZMAN J.A., HORTA D., HSIEH B.-C., HSU C.-H., HSU Y.-H., HUBER D., HUERTAS-COMPANY M., HUTCHINSON B., HWANG H.S., IBARRA-MEDEL H.J., IDER CHITHAM J., ILHA G.S., IMIG J., JAEKLE W., JAYASINGHE T., JI X., JOHNSON J.A., JONES A., JONSSON H., KATKOV I., KHALATYAN A., KINEMUCHI K., KISKU S., KNAPEN J.H., KNEIB J.-P., KOLLMEIER J.A., KONG M., KOUNKEL M., KRECKEL K., KRISHNARAO D., LACERNA I., LANE R.R., LANGGIN R., LAVENDER R., LAW D.R., LAZARZ D., LEUNG H.W., LEUNG H.-H., LEWIS H.M., LI C., LI R., LIAN J., LIANG F.-H., LIN L., LIN Y.-T., LIN S., LINTOTT C., LONG D., LONGA-PENA P., LOPEZ-COBA C., LU S., LUNDGREN B.F., LUO Y., MACKERETH J.T., DE LA MACORRA A., MAHADEVAN S., MAJEWSKI S.R., MANCHADO A., MANDEVILLE T., MARASTON C., MARGALEF-BENTABOL B., MASSERON T., MASTERS K.L., MATHUR S., McDERMID R.M., McKAY M., MERLONI A., MERRIFIELD M., MESZAROS S., MIGLIO A., DI MILLE F., MINNITI D., MINSLEY R., MONACHESI A., MOON J., MOSSER B., MULCHAEY J., MUNA D., MUNOZ R.R., MYERS A.D., MYERS N., NADATHUR S., NAIR P., NANDRA K., NEUMANN J., NEWMAN J.A., NIDEVER D.L., NIKAKHTAR F., NITSCHELM C., O'CONNELL J.E., GARMA-OEHMICHEN L., DE OLIVEIRA G.L.S., OLNEY R., ORAVETZ D., ORTIGOZA-URDANETA M., OSORIO Y., OTTER J., PACE Z.J., PADILLA N., PAN K., PAN H.-A., PARIKH T., PARKER J., PEIRANI S., PENA RAMIREZ K., PENNY S., PERCIVAL W.J., PEREZ-FOURNON I., PINSONNEAULT M., POIDEVIN F., POOVELIL V.J., PRICE-WHELAN A.M., QUEIROZ A.B.A., RADDICK M.J., RAY A., REMBOLD S.B., RIDDLE N., RIFFEL R.A., RIFFEL R., RIX H.-W., ROBIN A.C., RODRIGUEZ-PUEBLA A., ROMAN-LOPES A., ROMAN-ZUNIGA C., ROSE B., ROSS A.J., ROSSI G., RUBIN K.H.R., SALVATO M., SANCHEZ S.F., SANCHEZ-GALLEGO J.R., SANDERSON R., SANTANA ROJAS F.A., SARCENO E., SARMIENTO R., SAYRES C., SAZONOVA E., SCHAEFER A.L., SCHIAVON R., SCHLEGEL D.J., SCHNEIDER D.P., SCHULTHEIS M., SCHWOPE A., SERENELLI A., SERNA J., SHAO Z., SHAPIRO G., SHARMA A., SHEN Y., SHETRONE M., SHU Y., SIMON J.D., SKRUTSKIE M.F., SMETHURST R., SMITH V., SOBECK J., SPOO T., SPRAGUE D., STARK D.V., STASSUN K.G., STEINMETZ M., STELLO D., STONE-MARTINEZ A., STORCHI-BERGMANN T., STRINGFELLOW G.S., STUTZ A., SU Y.-C., TAGHIZADEH-POPP M., TALBOT M.S., TAYAR J., TELLES E., TESKE J., THAKAR A., THEISSEN C., TKACHENKO A., THOMAS D., TOJEIRO R., HERNANDEZ TOLEDO H., TROUP N.W., TRUMP J.R., TRUSSLER J., TURNER J., TUTTLE S., UNDA-SANZANA E., VAZQUEZ-MATA J.A., VALENTINI M., VALENZUELA O., VARGAS-GONZALEZ J., VARGAS-MAGANA M., VERA ALFARO P., VILLANOVA S., VINCENZO F., WAKE D., WARFIELD J.T., WASHINGTON J.D., WEAVER B.A., WEIJMANS A.-M., WEINBERG D.H., WEISS A., WESTFALL K.B., WILD V., WILDE M.C., WILSON J.C., WILSON R.F., WILSON M., WOLF J., WOOD-VASEY W.M., YAN R., ZAMORA O., ZASOWSKI G., ZHANG K., ZHAO C., ZHENG Z., ZHENG Z., ZHU K.
	Astrophys. J., Suppl. Ser., 259, 35-35 (2022)
	The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data.
o	<AP JHHMMSSss+DDMMSSs>.
=E=	Catalogue in electronic form as <III/284/>
=E=	Catalogue in electronic form as <III/286/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Ap
Ap	(Apriamaswili)
Write:	<<PN Ap 1-NN>> <<PN Ap 2-NN>> <<PN Ap 3-NN>> <<PN Ap 4-NN>> <<PN Ap 5-NN>>
N:	12+1+1+1+1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	5 lists: format 1-NN, 2-N, 3-N, 4-N, 5-N Ap 5-1 is not a PN
Ref:	=1962AZh....39..256F
by	FRANZMAN Y.L.
	Astron. Zh., 39, 256-259 (1962)
	A determination of the coordinates of planetary nebulae from photographs taken with an objective prism.
o	<PN Ap 1-NN> (Nos 1-1 to 1-12).
Ref:	=1962ATsir.231...25A
by	APRIAMASHVILI S.P.
	Astron. Tsirk., 231, 25-None (1962)
	A new planetary nebula.
o	<PN Ap 2-N> (No. 1).
Ref:	=1962ATsir.232....3A
by	APRIAMASHVILI S.P.
	Astron. Tsirk., 232, 3-None (1962)
	A new planetary nebula.
o	<PN Ap 3-N> (No. 1).
Ref:	=1964ATsir.279....1A
by	APRIAMASHVILI S.P.
	Astron. Tsirk., 279, 1-None (1964)
	A new planetary nebula.
o	<PN Ap 4-N> (No. 1).
Details on Acronym: AP
AP	(Arecibo obs., Pulsar)
Note:	Superseded by PSR
*****	Avoid the usage of AP, prefer PSR
Details on Acronym: [AP74]
[AP74]	(Austin+Peach, 1974) (Not yet in Simbad)
Write:	<<[AP74] NNN>>
N:	135
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	See also [AGP75], BGP, GP, [GP82]
in source:	ACO 1413
Ref:	=1974MNRAS.168..591A
by	AUSTIN T.B. , PEACH J.V.
	Mon. Not. R. Astron. Soc., 168, 591-602 (1974)
	Studies of rich clusters of galaxies. II. The structure and luminosity function of the cluster A1413.
o	Table I: <[AP74] NNN> (Nos 1-135)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AP97]
[AP97]	(Aguero+Paolantonio, 1997)
Write:	<<[AP97] NN>>
N:	12
Object:	Region (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Broadband BVRI observations at the 2.15m Ritchey-Chretien telescope of CASLEO, Argentina. Condensations or star-forming regions in NGC 1487.
in source:	NGC 1487
Ref:	=1997AJ....114..102A
by	AGUERO E.L. , PAOLANTONIO S.
	Astron. J., 114, 102-106 (1997)
	The peculiar galaxy NGC 1487.
o	Table 3: <[AP97] NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [APA2006]
[APA2006]	(Alonso-Herrero+Perez-Gonzalez+Alexander+, 2006)= (MIPS24)
Write:	<<[APA2006] MIPS24 NNNNNN>>
N:	92+21
Object:	IR G (SIMBAD class: Galaxy)
Note:	Spitzer MIPS 24mu.m selected galaxies in the CDFS.
in source:	NAME CDFS
Ref:	=2006ApJ...640..167A
by	ALONSO-HERRERO A. , PEREZ-GONZALEZ P.G., ALEXANDER D.M., RIEKE G.H., RIGOPOULOU D., LE FLOC'H E., BARMBY P., PAPOVICH C., RIGBY J.R., BAUER F.E., BRANDT W.N., EGAMI E., WILLNER S.P., DOLE H., HUANG J.-S.
	Astrophys. J., 640, 167-184 (2006)
	Infrared power-law galaxies in the Chandra Deep Field-South: active galactic nuclei and ultraluminous infrared galaxies.
o	Table 1: <[APA2006] MIPS24 NNNNNN> N=92 among (Nos 00243-013589).
Ref:	=2006ApJ...645..199S
by	SHI Y. , RIEKE G.H., PAPOVICH C., PEREZ-GONZALEZ P.G., LE FLOC'H E.
	Astrophys. J., 645, 199-208 (2006)
	Morphology of Spitzer 24 µm detected galaxies in the UDF: the links between star formation and galaxy morphology.
o	Table 1: <[APA2006] MIPS24 NNNNNN> N=21 added among (Nos 4641-15943).
=E=	Catalogue in electronic form as J/ApJ/640/167
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: APASS
APASS	(AAVSO Photometric All-Sky Survey)
Write:	<<APASS JDDD.dddd+DD.dddd>>
N:	about 55.10⁶
Object:	* (SIMBAD class: Star)
Note:	The AAVSO Photometric All-Sky Survey uses twin astrographs with CCD cameras that will cover the entire sky in five bandpasses: Johnson B and V, along with Sloan g,r,i. For more information, visit: http://www.aavso.org/apass
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [APB2016]
[APB2016]	(Alberts+Pope+Brodwin+, 2016)
Write:	<<[APB2016] JHHMMSS.s+DDMMSS>>
N:	129
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Herschel PACS photometric observations of N=129 galaxies in N=11 galaxy clusters at 1<z<1.75.
Ref:	=2016ApJ...825...72A
by	ALBERTS S. , POPE A., BRODWIN M., CHUNG S.M., CYBULSKI R., DEY A., EISENHARDT P.R.M., GALAMETZ A., GONZALEZ A.H., JANNUZI B.T., STANFORD S.A., SNYDER G.F., STERN D., ZEIMANN G.R.
	Astrophys. J., 825, 72-72 (2016)
	Star formation and AGN activity in galaxy clusters from z=1-2: a multi-wavelength analysis featuring Herschel/PACS.
o	Table 3: <[APB2016] JHHMMSS.s+DDMMSS> N=129.
=E=	Catalogue in electronic form as J/ApJ/825/72
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [APB2019]
[APB2019]	(Alcalde Pampliega+Perez-Gonzalez+Barro+, 2019)
Write:	<<[APB2019] GDW BBGNN>>
N:	33
Object:	Balmer Break G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=33 Balmer break galaxies (BBGs) selected as HST F160W droupouts in the deepest CANDELS/GOODS fields (H≳27.3mag) but relatively bright in Spitzer IRAC([3.6], [4.5]<24.5mag).
in source:	NAME GOODS North Field
in source:	NAME GOODS South Field
Ref:	=2019ApJ...876..135A
by	ALCALDE PAMPLIEGA B. , PEREZ-GONZALEZ P.G., BARRO G., DOMINGUEZ SANCHEZ H., ELICHE-MORAL M.C., CARDIEL N., HERNAN-CABALLERO A., RODRIGUEZ-MUNOZ L., SANCHEZ BLAZQUEZ P., ESQUEJ P.
	Astrophys. J., 876, 135-135 (2019)
	Optically faint massive Balmer break galaxies at z > 3 in the CANDELS/GOODS fields.
o	Tables 1+5+7: <[APB2019] GDN BBGNN> (Nos GDN BBG01-GDN BBG17), <[APB2019] GDS BBGNN> (Nos GDS BBG01-GDS BBG16).
=E=	Catalogue in electronic form as <J/ApJ/876/135/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [APB76]
[APB76]	(Alloin+Pelat+Bijaoui, 1976) (Not yet in Simbad)
Write:	<<[APB76] {A\|B\|C}N>>
N:	8
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=8 objects sourounding the nuleus of M 31 within 140" of the center.
in source:	M 31 = NGC 224
Ref:	=1976A&A....50..127A
by	ALLOIN D. , PELAT D., BIJAOUI A.
	Astron. Astrophys., 50, 127-None (1976)
	Electronographic study of the nuclear region in M 31.
o	Fig.5, Table 2: <[APB76] AN> (Nos A, B1-B4, C1-C3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [APB90]
[APB90]	(Asatrian+Petrosian+Borngen, 1990)
Write:	<<[APB90] A>>
N:	4
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=4 galaxies around Mrk 273.
Ref:	=1990PAZh...16..495A
by	ASATRIAN A.S. , PETROSIAN A.R., BORNGEN F.
	Pis'ma Astron. Zh., 16, 495-None (1990)
	New data on peculiar galaxy MRK 273.
o	Fig.1: <[APB90] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [APC2003]
[APC2003]	(Astier+Pritchet+CFHT Legacy Survey+, 2003)= (LSSP)
Write:	<<[APC2003] JHHMMSS.ss+DDMMSS.s>>
N:	7+6+11+4
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxies of SN 2003FE to SN 2003FZ, SN 2003GA, SN 2003GB, SN 2003GY, SN 2003GZ, SN 2003HA, SN 2003HB.
Ref:	=2003IAUC.8147....2A
by	ASTIER P. , PRITCHET C., (The CFHT Legacy Survey Supernova Project), AUBOURG E., BALAM D., CARLBERG R., HARDIN D., GUIDE D., FABBRO S., LAFOUX H., MERRALL T., PAIN R., PERRETT K., RICH J., SCHAHMANECHE K., ANTILOGUS P., LESQUOY E., SAINTON G.
	IAU Circ., 8147, 2-None (2003)
	Supernovae 2003fe, 2003ff, 2003fg, 2003fh, 2003fi, 2003fj, 2003fk.
o	<[APC2003] JHHMMSS.ss+DDMMSS.s> N=7.
Ref:	=2003IAUC.8148....2A
by	ASTIER P. , PRITCHET C., (The CFHT Legacy Survey Supernova Project)
	IAU Circ., 8148, 2-None (2003)
	Supernovae 2003fl, 2003fm, 2003fn, 2003fo, 2003fp, 2003fq.
o	<[APC2003] JHHMMSS.ss+DDMMSS.s> N=6.
Ref:	=2003IAUC.8149....1A
by	ASTIER P. , PRITCHET C., (The CFHT Legacy Survey Supernova Project)
	IAU Circ., 8149, 1-None (2003)
	Supernovae 2003fr-2003gb.
o	<[APC2003] JHHMMSS.ss+DDMMSS.s> N=11.
Ref:	=2003IAUC.8178....2A
by	ASTIER P. , PRITCHET C., (The CFHT Legacy Survey Supernova Project), FOUCHEZ D., RAUX J.
	IAU Circ., 8178, 2-None (2003)
	Supernovae 2003gy, 2003gz, 2003ha, 2003hb.
o	<[APC2003] JHHMMSS.ss+DDMMSS.s> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [APD2000]
[APD2000]	(Andreon+Pello+Davoust+, 2000)
Write:	<<[APD2000] JHHMMSS.s+DDMMSS>>
N:	77+124+88
Object:	(Near IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	Coma Cluster = ACO 1656
Ref:	=2000A&AS..141..113A
by	ANDREON S. , PELLO R., DAVOUST E., DOMINGUEZ R., POULAIN P.
	Astron. Astrophys., Suppl. Ser., 141, 113-122 (2000)
	Extensive near-infrared (H-band) photometry in Coma.
o	Tables 3, 4, 5: <[APD2000] JHHMMSS.s+DDMMSS> N=77+124+88.
=E=	Catalogue in electronic form as J/A+AS/141/113
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [APD2013]
[APD2013]	(Andersson+Piirola+De Buizer+, 2013)
Write:	<<[APD2013] IC63 #NN>>
Object:	* (SIMBAD class: Star)
Note:	NOT ALFOSC (spectro-polarimetry) and TURPOL (photo-polarimetry) observations of N=14 stars in IC 63.
in source:	IC 63
Ref:	=2013ApJ...775...84A
by	ANDERSSON B.-G. , PIIROLA V., DE BUIZER J., CLEMENS D.P., UOMOTO A., CHARCOS-LLORENS M., GEBALLE T.R., LAZARIAN A., HOANG T., VORNANEN T.
	Astrophys. J., 775, 84 (2013)
	Evidence for H_{2} formation driven dust grain alignment in IC 63.
o	Fig. 2, Tables 1-4: <[APD2013] IC63 #NN> N=14 among (Nos 5-76).
=E=	Catalogue in electronic form as <J/ApJ/775/84/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [APF2013]
[APF2013]	(An+Paragi+Frey+, 2013) (Not yet in Simbad)
Write:	<<[APF2013] WN>> <<[APF2013] CN>>
N:	7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	e-MERLIN and EVL 5GHz observations of N=7 compact components of 3C 316.
Ref:	=2013MNRAS.433.1161A
by	AN T. , PARAGI Z., FREY S., XIAO T., BAAN W.A., KOMOSSA S., GABANYI K.E., XU Y.-H., HONG X.-Y.
	Mon. Not. R. Astron. Soc., 433, 1161-1171 (2013)
	The radio structure of 3C 316, a galaxy with double-peaked narrow optical emission lines.
o	Fig. 1, Table 1: <[APF2013] AN> (Nos E1-E3, W1, C1-C3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: APG
APG	(Atlas of Peculiar G)= (A) = Arp
Write:	<<APG NNNA>>
N:	338+?
Object:	G (SIMBAD class: Galaxy)
Ref:	=1966ApJS...14....1A
by	ARP H.
	Astrophys. J., Suppl. Ser., 14, 1-20 (1966)
	Atlas of peculiar galaxies.
o	<APG NNN> (Nos 1-338).
Ref:	=1983ApJ...270..465S
by	STAUFFER J. , SCHILD R., KEEL W.
	Astrophys. J., 270, 465-470 (1983)
	ARP 102B : a new and unusual broad-line galaxy.
o	<APG NNNA> N=2, Nos 102A, B. 1st ref. with this format
=E=	Catalogue in electronic form as VII/74
Details on Acronym: [APG2008]
[APG2008]	(Allen+Pipher+Gutermuth+, 2008)
Write:	<<[APG2008] JHHMMSS.ss+DDMMSS.ss>>
N:	19+74+6+20
Object:	(Near IR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	KPNO 2.1m telescope NIR and Spitzer IRAC observations of the young cluster [C86] L988 e.
in source:	[C86] L988 e
Ref:	=2008ApJ...675..491A
by	ALLEN T.S. , PIPHER J.L., GUTERMUTH R.A., MEGEATH S.T., ADAMS J.D., HERTER T.L., WILLIAMS J.P., GOETZ-BIXBY J.A., ALLEN L.E., MYERS P.C.
	Astrophys. J., 675, 491-506 (2008)
	Spitzer, near-infrared, and submillimeter imaging of the relatively sparse young cluster, Lynds 988e.
o	Lynds 988e = NAME [C86] L988 e CLUSTER in SIMBAD.
o	Tables 2-5: <[APG2008] JHHMMSS.ss+DDMMSS.ss> N=19+74+6+20.
=E=	Catalogue in electronic form as J/ApJ/675/491
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [APH2018]
[APH2018]	(Arrigoni Battaia+Prochaska+Hennawi+, 2018)
Write:	<<[APH2018] SDSS J1020+1040 nebula>> <<[APH2018] AGN1>> <<[APH2018] QSO2>> <<[APH2018] LAEN>>
N:	1+4
Object:	Protocluster + AGN + Em. Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT MUSE observations N=1 enormous Ly α nebula, N=2 AGN and N=2 Ly α emiiters in the field of the SDSS J102009.99+104002.7 quasar. See also [CAP2014] and [HPC2015].
Ref:	=2018MNRAS.473.3907A
by	ARRIGONI BATTAIA F. , PROCHASKA J.X., HENNAWI J.F., OBREJA A., BUCK T., CANTALUPO S., DUTTON A.A., MACCIO A.V.
	Mon. Not. R. Astron. Soc., 473, 3907-3940 (2018)
	Inspiraling halo accretion mapped in Ly α emission around a z ~ 3 quasar.
o	Table 1: <[APH2018] QSO2> N=1, <[APH2018] AGN1> N=1, <[APH2018] LAEN> (Nos 1-2). Text: <[APH2018] SDSS J1020+1040 nebula> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ApM
ApM	(Arp+Madore)
*****	Avoid the usage of ApM, prefer AM
Details on Acronym: APM
APM	(Automatic Plate Measuring machine)
*****	Avoid the usage of APM, prefer APMBGC
Origin	of the Acronym: L = Found in the literature
Details on Acronym: APM
APM	(Automatic Plate Measuring machine)
*****	Avoid the usage of APM, prefer APMGS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: APM
APM	(Automatic Plate Measuring)
*****	Avoid the usage of APM, prefer DKI
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [APM2014]
[APM2014]	(Allen+Prchlik+Megeath+, 2014) (Not yet in Simbad)
Write:	<<[APM2014] NN>>
N:	76
Object:	K giant (SIMBAD class: Star)
Note:	MMT Hectospec spectroscopy of N=76 K giant stars to determine the extinction law through Cep OB3b. Use of SDSS DR9 and 2MASS data.
in source:	NAME Ass Cep OB 3b
Ref:	=2014ApJ...786..113A
by	ALLEN T.S. , PRCHLIK J.J., MEGEATH S.T., GUTERMUTH R.A., PIPHER J.L., NAYLOR T., JEFFRIES R.D.
	Astrophys. J., 786, 113 (2014)
	An anomalous extinction law in the Cep OB3b young cluster: evidence for dust processing during gas dispersal.
o	Table 1: <[APM2014] NN> (Nos 1-76).
=E=	Catalogue in electronic form as <J/ApJ/786/113/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: APMBGC
APMBGC	(Automatic Plate Measuring machine, Bright Galaxy Catalogue)= (APM)
Write:	<<APMBGC FFF+xxx+yyy>>
N:	15827
Object:	G (SIMBAD class: Galaxy)
Note:	Format 'FFF+xxx+yyy': 'FFF' stands for the SERC field number '+xxx+yyy' stands for the position of the galaxy on the plate, in millimetres from the centre of the plate. These are preceded by a sign for the galaxy position in the plate: '+' sign for the galaxy to the right (west) of the centre (+xxx) below (south) of the centre (+yyy) '-' sign for the galaxy to the left (east) of the centre (-xxx) above (north) of the centre of the plate (-yyy)
Ref:	=1996MNRAS.278.1025L
by	LOVEDAY J.
	Mon. Not. R. Astron. Soc., 278, 1025-1048 (1996)
	The APM Bright Galaxy Catalogue.
o	<APMBGC FFF+xxx+yyy> N=14681
Ref:	=1996ApJS..107..201L
by	LOVEDAY J. , PETERSON B.A., MADDOX S.J., EFSTATHIOU G.
	Astrophys. J., Suppl. Ser., 107, 201-214 (1996)
	The Stromlo-APM redshift survey. IV. The redshift catalog.
o	<APMBGC FFF+xxx+yyy> N=1797 (1147 added).
=E=	Catalogue in electronic form as J/MNRAS/278/1025
=E=	Catalogue in electronic form as J/ApJS/107/201
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: APMBGS
APMBGS	(Automatic Plate Measuring machine, Bright Galaxy Survey)
*****	Avoid the usage of APMBGS, prefer APMGS
Origin	of the Acronym: L = Found in the literature
Details on Acronym: APMC
APMC	(Automatic Plate Measuring machine, Cluster)
*****	Avoid the usage of APMC, prefer APMCC
Origin	of the Acronym: L (1998ApJ...506..509K)
Details on Acronym: APMCC
APMCC	(Automatic Plate Measuring machine, Cluster Catalogue)= APMC = ([DMS97])
Write:	<<APMCC NNN>>
N:	957
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	See also [DEM94]
Ref:	=1997MNRAS.289..263D
by	DALTON G.B. , MADDOX S.J., SUTHERLAND W.J., EFSTATHIOU G.
	Mon. Not. R. Astron. Soc., 289, 263-284 (1997)
	The APM galaxy survey - V. Catalogues of galaxy clusters.
o	Table A1: <APMCC NNN> (Nos 1-957)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: APMGS
APMGS	(Automatic Plate Measuring machine, Galaxy Survey)= (APM) = APMBGS
Write:	<<APMGS HHMMSS.s+DDMMSS>> <<APMGS HHMMSS.s+DDMMSS.s>> <<APMGS HHMMSS.ss+DDMMSS.s>>
Object:	G (SIMBAD class: Galaxy)
Ref:	=1990MNRAS.246..433M
by	MADDOX S.J. , EFSTATHIOU G., SUTHERLAND W.J.
	Mon. Not. R. Astron. Soc., 246, 433-457 (1990)
	The APM galaxy survey. II. Photometric corrections.
o	Table 3: <APMGS HHMMSS.s-DDMMSS> N=266
Ref:	=1994MNRAS.269..151D
by	DALTON G.B. , EFSTATHIOU G., MADDOX S.J., SUTHERLAND W.J.
	Mon. Not. R. Astron. Soc., 269, 151-165 (1994)
	The APM galaxy survey. IV. Redshifts of rich clusters of galaxies.
o	(Erratum) erratum vol. 273 p.528
o	Table 3: <APMGS HHMMSS.ss-DDMMSS.s> N=365. Tables 1, 2, 4: <[DEM94] HHMMSS.s-DDMMSS> N=228
Ref:	=1995AJ....110.1032M
by	MURIEL H. , NICOTRA M.A., LAMBAS D.G.
	Astron. J., 110, 1032-1038 (1995)
	The luminosity function of elliptical galaxies.
o	<APMGS HHMMSS.s-DDMMSS.s> N=292
=E=	Catalogue in electronic form as J/MNRAS/246/433
=E=	Catalogue in electronic form as J/MNRAS/269/151
=E=	Catalogue in electronic form as J/AJ/110/1032
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: APMPM
APMPM	(Automatic Plate Measuring machine, PM*)
Write:	<<APMPM JHHMM+DDMMA>>
Object:	PM* (SIMBAD class: HighPM* = High Proper Motion Star)
Note:	PM* observed with the APM. Format 'JHHMM+DDMM', and JHHMM+DDMMA' for components of a common PM*. First refs with an 'APMPM' designation.
Ref:	=1997MNRAS.292L..41G
by	GIZIS J.E. , SCHOLZ R.-D., IRWIN M., JAHREISS H.
	Mon. Not. R. Astron. Soc., 292, 41-43 (1997)
	APMPM J1523-0245: a new high proper motion cool subdwarf.
o	<APMPM JHHMM+DDMM> N=1.
Ref:	=1999A&A...345L..55S
by	SCHOLZ R.-D. , IRWIN M., SCHWEITZER A., IBATA R.
	Astron. Astrophys., 345, 55-57 (1999)
	APMPM J0237-5928: a new nearby active M5 dwarf detected in a high proper motion survey of the Southern sky.
o	<APMPM JHHMM+DDMM> N=1.
Ref:	=1999A&A...350L..62S
by	SCHWEITZER A. , SCHOLZ R.-D., STAUFFER J., IRWIN M., McCAUGHREAN M.J.
	Astron. Astrophys., 350, 62-64 (1999)
	APMPM J0559-2903: The coolest extreme subdwarf known.
o	<APMPM JHHMM+DDMM> N=1.
Ref:	=2000A&A...353..958S
by	SCHOLZ R.-D. , IRWIN M., IBATA R., JAHREISS H., MALKOV O.Y.
	Astron. Astrophys., 353, 958-969 (2000)
	New high-proper motion survey in the Southern sky.
o	Catalogue, col(1): <[SII2000] NNN> (Nos 1-204), = col(3): <APMPM JHHMM+DDMMA> N=204.
Ref:	=2002A&A...390..491R
by	REYLE C. , ROBIN A.C., SCHOLZ R.-D., IRWIN M.
	Astron. Astrophys., 390, 491-499 (2002)
	New nearby stars selected in a high proper motion survey by DENIS photometry.
o	Table 1: <APMPM JHHMM+DDMM> N=147.
=E=	Catalogue in electronic form as J/A+A/390/491
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: APMS
APMS	(Automatic Plate Measuring machine, Supercluster)
Write:	<<APMS NN>>
N:	16 among 83
Object:	Supercluster of G (SIMBAD class: SuperClG = Supercluster of Galaxies)
Note:	Table 3: N=16 superclusters among 83 with 3 or more galaxies found in the APM survey.
Ref:	=1998ApJ...506..509K
by	KALINKOV M. , VALTCHANOV I., KUNEVA I.
	Astrophys. J., 506, 509-518 (1998)
	Correlation function of superclusters of galaxies.
o	Table 1: 'T NN' from Thuan, 1980, not in SIMBAD.
o	Table 3: <APMS NN> N=16 among 83.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: APMSCC
APMSCC	(APM, Super Cluster Catalogue)
Write:	<<APMSCC NN>>
N:	55
Object:	Supercluster of G (SIMBAD class: SuperClG = Supercluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Catalogue of supercluster of galaxies, from the APM catalogue of clusters APMCC.
Ref:	=2002AJ....123...51E
by	EINASTO M. , EINASTO J., TAGO E., ANDERNACH H., DALTON G.B., MUELLER V.
	Astron. J., 123, 51-65 (2002)
	Optical and X-ray clusters as tracers of the supercluster-void network. III. Distribution of Abell and APM clusters.
o	Table A1: <APMSCC NN> (Nos 1-55).
=E=	Catalogue in electronic form as J/AJ/123/51
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: APMUKS
APMUKS	(APM+UKS)
Write:	<<APMUKS (BJ) BHHMMSS.ss+DDMMSS.s>>
N:	3946067
Object:	G (SIMBAD class: Galaxy)
Note:	Description of the catalogue in 1990MNRAS.243..692M In the format (end of the acronym for the authors), (BJ) stands for B,J filter.
Ref:	=1990MNRAS.243..692M
by	MADDOX S.J. , SUTHERLAND W.J., EFSTATHIOU G., LOVEDAY J.
	Mon. Not. R. Astron. Soc., 243, 692-712 (1990)
	The APM galaxy survey - I. APM measurements and star-galaxy separation.
o	Description of the catalogue, no object
o	<APMUKS (BJ) BHHMMSS.ss+DDMMSS.s> N=3946067
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: APMUKS(BJ)
APMUKS(BJ)	(APM+UKS, B,J filter)
*****	Avoid the usage of APMUKS(BJ), prefer APMUKS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: APOGEE
APOGEE	(APO Galactic Evolution Experiment)
*****	Avoid the usage of APOGEE, prefer AP
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: APOP
APOP	(Absolute Proper motions Outside the Plane)
Write:	<<APOP NNNNN+NNNNNNN>>
N:	100774153
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	A new catalog of absolute proper motions and updated positions derived from the same Space Telescope Science Institute digitized Schmidt survey plates utilized for the construction of the Guide Star Catalog II. The catalog covers 22,525 sq. degrees and lists N=100774153 objects to the limiting magnitude of R_F∼20.8.
Ref:	=2015AJ....150..137Q
by	QI Z. , YU Y., BUCCIARELLI B., LATTANZI M.G., SMART R.L., SPAGNA A., McLEAN B.J., TANG Z., JONES H.R.A., MORBIDELLI R., NICASTRO L., VECCHIATO A.
	Astron. J., 150, 137 (2015)
	Absolute proper motions outside the plane (APOP)-a step toward the GSC2.4.
o	<APOP NNNNN+NNNNNNN> N=100774150.
=E=	Catalogue in electronic form as <I/331/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [APP2021]
[APP2021]	(Aoki+Primas+Pasquini+, 2021)
Write:	<<[APP2021] NNNNNN>>
N:	316
Object:	* (SIMBAD class: Star)
Note:	N=316 stars in NGC 104, using archival VLT FLMAES/GIRAFFE data.
in source:	47 Tuc = NGC 104
Ref:	=2021A&A...653A..13A
by	AOKI M. , PRIMAS F., PASQUINI L., WEISS A., SALARIS M., CAROLLO D.
	Astron. Astrophys., 653A, 13-13 (2021)
	Lithium in NGC 2243 and NGC 104.
o	Table 2: <[APP2021] NNNNNN> N=316 among (Nos 429-213017).
=E=	Catalogue in electronic form as <J/A+A/653/A13/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: APPLES
APPLES	(ACS Pure Parallel Ly-alpha Emission Survey)
Write:	<<NAME APPLES N>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Note:	HST ACS APPLES first object discovered. See also [PLF2005].
Ref:	=2005AJ....129..148P
by	PASQUALI A. , LARSEN S., FERRERAS I., GNEDIN O.Y., MALHOTRA S., RHOADS J.E., PIRZKAL N., WALSH J.R.
	Astron. J., 129, 148-159 (2005)
	Discovery of a solitary dwarf galaxy in the APPLES survey.
o	<NAME APPLES 1>. Fig.6: <[PLF2005] N> (Nos 1-3).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [APR2004]
[APR2004]	(Alonso-Herrero+Perez-Gonzalez+Rigby+, 2004)
Write:	<<[APR2004] DDD.dddddd+DD.dddddd>>
N:	29
Object:	G (SIMBAD class: Galaxy)
Note:	Spitzer Space Telescope observations of X-ray selected sources in the extended Groth strip. DDD.dddddd+DD.dddddd is the position from Chandra.
Ref:	=2004ApJS..154..155A
by	ALONSO-HERRERO A. , PEREZ-GONZALEZ P.G., RIGBY J., RIEKE G.H., LE FLOC'H E., BARMBY P., PAGE M.J., PAPOVICH C., DOLE H., EGAMI E., HUANG J.-S., RIGOPOULOU D., CRISTOBAL-HORNILLOS D., ELICHE-MORAL C., BALCELLS M., PRIETO M., ERWIN P., ENGELBRACHT C.W., GORDON K.D., WERNER M., WILLNER S.P., FAZIO G.G., FRAYER D., HINES D., KELLY D., LATTER W., MISSELT K., MIYAZAKI S., MORRISON J., RIEKE M.J., WILSON G.
	Astrophys. J., Suppl. Ser., 154, 155-159 (2004)
	The nature of luminous X-ray sources with mid-infrared counterparts.
o	Table 1: <[APR2004] DDD.dddddd+DD.dddddd> N=29.
=E=	Catalogue in electronic form as J/ApJS/154/155
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Apriamasvili
Apriamasvili	(Apriamasvili)
*****	Avoid the usage of Apriamasvili, prefer Apriamaswili
Details on Acronym: Apriamaswili
Apriamaswili	(Apriamasvili)= Apriamasvili
Write:	<<Cl Apriamaswili N>>
N:	1
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Stat:	is completely incorporated in Simbad
Ref:	=1964ATsir.280....1A
by	APRIAMASHVILI S.P.
	Astron. Tsirk., 280, 1-2 (1964)
	On a new open cluster in Scutum.
o	<Cl Apriamaswili N> (No. 1).
Details on Acronym: APS
APS	(Automated Plate Scanner)
*****	Avoid the usage of APS, prefer MAPS
Origin	of the Acronym: L (2000A&A...355..461A)
Details on Acronym: [APS2006]
[APS2006]	(Adami+Picat+Savine+, 2006)
Write:	<<[APS2006] NNNNN>>
N:	60588
Object:	* + G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	CFHT CFH12K observations of the Coma Cluster. The numbering NNNNN (Nos 1-60588), not present in the published catalog, represents the running number of the star in the catalog ('recno' number in the catalog J/A+A/451/1159).
in source:	Coma Cluster = ACO 1656
Ref:	=2006A&A...451.1159A
by	ADAMI C. , PICAT J.P., SAVINE C., MAZURE A., WEST M.J., CUILLANDRE J.-C., PELLO R., BIVIANO A., CONSELICE C.J., DURRET F., GALLAGHER III J.S., GREGG M., MOREAU C., ULMER M.
	Astron. Astrophys., 451, 1159-1170 (2006)
	Deep and wide field imaging of the Coma cluster: the data.
o	The numbering used in SIMBAD, with the agreement of authors, is not present in the published catalog, but represents the running number of the star in the catalog ('recno' number in the catalog J/A+A/451/1159)
o	Catalog: <[APS2006] NNNNN> (Nos 1-60588).
=E=	Catalogue in electronic form as J/A+A/451/1159
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [APS2019]
[APS2019]	(Amado+Povic+Sanchez-Portal+, 2019)
Write:	<<[APS2019] NNN>>
N:	231
Object:	G in ClG (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=231 cluster galaxies in ZwCl 0024+1652. Use of HST data.
in source:	HMS 0024+1654 = ClG 0024+1652
Ref:	=2019MNRAS.485.1528A
by	AMADO Z.B. , POVIC M., SANCHEZ-PORTAL M., TESSEMA S.B., BONGIOVANNI A., CEPA J., CERVINO M., GONZALEZ-SERRANO J.I., NADOLNY J., PEREZ GARCIA A.M., PEREZ-MARTINEZ R., PINTOS-CASTRO I.
	Mon. Not. R. Astron. Soc., 485, 1528-1545 (2019)
	A morphological study of galaxies in ZwCl0024+1652, a galaxy cluster at redshift z ~ 0.4.
o	Table A1: <[APS2019] NNN> (Nos 1-231).
=E=	Catalogue in electronic form as <J/MNRAS/485/1528/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: APTF
APTF	(Apertif continuum source catalog)
Write:	<<APTF JHHMMSS+DDMMSS>>
N:	>100000
Object:	Radio source (SIMBAD class: Radio = Radio Source)
Note:	Apertif continuum survey is a wide field survey at 1.4 GHz. It was performed during 2019-2022 and covered approximately 2300 square degrees. The data releases of Apertif can be found at https://vo.astron.nl
Ref:	=2022A&A...667A..39K
by	KUTKIN A.M. , OOSTERLOO T.A., MORGANTI R., ADAMS E.A.K., MANCINI M., ADEBAHR B., DE BLOK W.J.G., DENES H., HESS K.M., VAN DER HULST J.M., LUCERO D.M., MOSS V.A., BERGER A., VAN DEN BRINK R., VAN CAPPELLEN W.A., CONNOR L., DAMSTRA S., LOOSE G.M., VAN LEEUWEN J., MAAN Y., MIKA A., NORDEN M.J., OFFRINGA A.R., OOSTRUM L.C., VAN DER SCHUUR D., VOHL D., WIJNHOLDS S.J., ZIEMKE J.
	Astron. Astrophys., 667A, 39 (2022)
	Continuum source catalog for the first APERTIF data release.
o	Table 1: <APTF JHHMMSS+DDMMSS> N=249672. ASTRON
=E=	Catalogue in electronic form as <J/A+A/667/A39/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: APX
APX	(Alpha Persei, X-ray source)
Write:	<<APX NNN>> <<APX NNNA>>
N:	203+656
Object:	(X) + * (SIMBAD class: X = X-ray Source)
Note:	ROSAT PSPC observations of the alpha Persei Cluster = Cl Melotte 20. (Nos 1-203) X-ray sources detected. Format 'NNNA' are possible optical counterparts. Finding charts. See also Cl* Melotte 20 AP.
in source:	NAME ALPHA PER Cluster
Ref:	=1998AN....319..201P
by	PROSSER C.F. , RANDICH S.
	Astron. Nachr., 319, 201-214 (1998)
	Identification of new low-mass members of the α Persei open cluster by ROSAT. I.
o	Table 1: <APX NN> (Nos 1-73). Table 2, notes finding charts: <APX NNA> N=88.
Ref:	=1998AN....319..215P
by	PROSSER C.F. , RANDICH S., SIMON T.
	Astron. Nachr., 319, 215-234 (1998)
	Identification of new low-mass members of the α Persei open cluster by ROSAT. II.
o	Table 2: <APX NNN> (Nos 74-203). Tables 4, 7: <APX NNNA> N=568.
=E=	Catalogue in electronic form as J/other/AN/319.201
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Aq
Aq	(Aquarius)
*****	Avoid the usage of Aq, prefer [SDM2004]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Aql
Aql	(Aquila)
*****	Avoid the usage of Aql, prefer [P69]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Aqr
Aqr	(Aquarius field) (Not yet in Simbad)
*****	Avoid the usage of Aqr, prefer [CP83b]
Details on Acronym: AqrCC
AqrCC	(Aquarius, Cluster Catalog)
Write:	<<AqrCC NNN>>
N:	102
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	See also [CMK2002]. Paper II: [CMW2004].
Ref:	=2002AJ....123.1200C
by	CARETTA C.A. , MAIA M.A.G., KAWASAKI W., WILLMER C.N.A.
	Astron. J., 123, 1200-1215 (2002)
	The Aquarius superclusters. I. Identification of clusters and superclusters.
o	Table 2: <[CMK2002] Gal N> (Nos 1-5). Table 3: <AqrCC NNN> (Nos 1-102).
=E=	Catalogue in electronic form as J/AJ/123/1200
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AR
AR	(Absoption Region) (Not yet in Simbad)
*****	Avoid the usage of AR, prefer [H73]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AR
AR	(Arches Radio)
*****	Avoid the usage of AR, prefer [LGR2001]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AR2001]
[AR2001]	(Arp+Russell, 2001) (Not yet in Simbad)
Write:	<<[AR2001] N>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT PSPC X-ray sources (Nos 1-3) flanking the central galaxy ESO 185-54.
Ref:	=2001ApJ...549..802A
by	ARP H. , RUSSELL D.
	Astrophys. J., 549, 802-819 (2001)
	A possible relationship between quasars and clusters of galaxies.
o	Fig.4: <[AR2001] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AR2002]
[AR2002]	(Anglada+Rodriguez, 2002)
Write:	<<[AR2002] L1448 IRS 2 VLA N>> <<[AR2002] AFGL-iki VLA N>> <<[AR2002] IRAS HHMMm+DDMM VLA N>> <<[AR2002] NGC 2023 mm1 VLA N>> <<[AR2002] LNNNN VLA N>>
N:	33
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA observations of 9 fields containing molecular outflows.
Ref:	=2002RMxAA..38...13A
by	ANGLADA G. , RODRIGUEZ L.F.
	Rev. Mex. Astron. Astrofis., 38, 13-21 (2002)
	VLA detection of the exciting sources of the molecular outflows associated with L1448 IRS2, IRAS 05327+3404, L43, IRAS 22142+5206, L1211, and IRAS 23545+6508.
o	Table 2: <[AR2002] L1448 IRS 2 VLA N> (Nos 1-6), <[AR2002] AFGL-iki VLA N> (Nos 1-2), <[AR2002] IRAS 05327+3404 VLA N> (Nos 1-2), <[AR2002] NGC 2023 mm1 VLA N> (Nos 1-2), <[AR2002] L43 VLA N> (Nos 1-4), <[AR2002] IRAS 22103+5828 VLA N> (Nos 1-3), <[AR2002] IRAS 22142+5206 VLA N> (Nos 1-2), <[AR2002] L1211 VLA N> (Nos 1-5), <[AR2002] IRAS 23545+6508 VLA N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AR86]
[AR86]	(Arsenault+Roy, 1986)
Write:	<<[AR86] NNNNNR>> <<[AR86] IC2574R>> <<[AR86] HOII-I>>
N:	27+2+1
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Mont Megantic 1.6m telescope and CFHT 3.6m telescope observations of HII regions in nearby galaxies.
Ref:	=1986AJ.....92..567A
by	ARSENAULT R. , ROY J.-R.
	Astron. J., 92, 567-579 (1986)
	Integrated H α profiles of giant extragalactic H II regions.
o	Table II: <[AR86] NNNNNR> N=27, <[AR86] IC2574R> (Nos I-II), <[AR86] HOII-I> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 92ar
92ar	(SN 1992ar)
*****	Avoid the usage of 92ar, prefer [CPS2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AR95]
[AR95]	(Anderson+Rudnick, 1996)
Write:	<<[AR95] NNN>>
N:	304
Object:	Knot (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
in source:	NAME Cas A
Ref:	=1995ApJ...441..307A
by	ANDERSON M.C. , RUDNICK L.
	Astrophys. J., 441, 307-333 (1995)
	The deceleration powering of synchrotron emission from ejecta components in supernova remnant Cassiopeia A.
o	Table 3: <[AR95] NNN> (Nos 1-304)
=E=	Catalogue in electronic form as J/ApJ/441/307
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ara
Ara	(Ara)
*****	Avoid the usage of Ara, prefer [MWC53]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Arak
Arak	(Arakelian)
*****	Avoid the usage of Arak, prefer Ark
Details on Acronym: Arakelian
Arakelian	(Arakelian)
*****	Avoid the usage of Arakelian, prefer Ark
Details on Acronym: Arakeljan
Arakeljan	(Arakelian)
*****	Avoid the usage of Arakeljan, prefer Ark
Details on Acronym: Arakelyan
Arakelyan	(Arakelian)
*****	Avoid the usage of Arakelyan, prefer Ark
Details on Acronym: [ARB2011]
[ARB2011]	(Armond+Reipurth+Bally+, 2011)
Write:	<<[ARB2011] MKHa NN>> <<[ARB2011] NIR NN>>
N:	30+25
Object:	H-alpha Em* + PMS* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	University of Hawaii 2.2m telescope and NASA IRTF observations of N=30 Hα emission-line stars and N=25 embedded PMS stars in the "Gulf of Mexico".
in source:	NAME GULF OF MEXICO = LDN 935
Ref:	=2011A&A...528A.125A
by	ARMOND T. , REIPURTH B., BALLY J., ASPIN C.
	Astron. Astrophys., 528A, 125-125 (2011)
	Star formation in the ``Gulf of Mexico''.
o	Table 3: <HH NNN> (Nos 952-958) added. Fig. 13, Table 4: <[ARB2011] MKHa NN> (Nos 1-30). Fig. 16, Table 5: <[ARB2011] NIR NN> (Nos 1-25).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ARB90]
[ARB90]	(Arsenault+Roy+Boulesteix, 1990)
Write:	<<[ARB90] NNN>>
N:	127
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	map
in source:	NGC 4321
Ref:	=1990A&A...234...23A
by	ARSENAULT R. , ROY J.-R., BOULESTEIX J.
	Astron. Astrophys., 234, 23-39 (1990)
	Large-scale formation of massive stars in the spiral galaxy NGC 4321.
o	<[ARB90] NNN> N=127
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ARC2001]
[ARC2001]	(Avila+Rodriguez+Curiel, 2001)
Write:	<<[ARC2001] HH NNN VLA N>>
N:	53
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA observations toward 10 HH objects regions. Maps in Figs 1 to 12.
Ref:	=2001RMxAA..37..201A
by	AVILA R. , RODRIGUEZ L.F., CURIEL S.
	Rev. Mex. Astron. Astrofis., 37, 201-211 (2001)
	VLA detection of the exciting sources of the HH 221 and HH 68 outflows.
o	in ref list ANGLADA 1995RMxAC.1.67 instead of 1.6, GEE at al 1985MNRAS. 215p.15 instead of 215.15
o	Table 2: <[ARC2001] HH NNN VLA N> N=53.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ARC2009]
[ARC2009]	(Ajello+Rebusco+Cappelluti+, 2009)= (Swift) (Not yet in Simbad)
Write:	<<[ARC2009] JHHMM.m+DDMM>>
N:	10
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Swift/BAT all-sky survey detection of clusters of galaxies.
Ref:	=2009ApJ...690..367A
by	AJELLO M. , REBUSCO P., CAPPELLUTI N., REIMER O., BOHRINGER H., GREINER J., GEHRELS N., TUELLER J., MORETTI A.
	Astrophys. J., 690, 367-388 (2009)
	Galaxy clusters in the Swift/Burst Alert Telescope era: hard X-rays in the intracluster medium.
o	Table 1: <[ARC2009] JHHMM.m+DDMM> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ARC92]
[ARC92]	(Anglada+Rodriguez+Canto+, 1992)
Write:	<<[ARC92] LDN 1524 N>> <<[ARC92] LDN 1527 N>> <<[ARC92] RNO 43 N>> <<[ARC92] Haro 4-255 FIR N>> <<[ARC92] AS 353A N>> <<[ARC92] Barn 335 NN>> <<[ARC92] PV Cep N>>
N:	35
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio-sources in the field of 7 YSO. See also [AVE98].
Ref:	=1992ApJ...395..494A
by	ANGLADA G. , RODRIGUEZ L.F., CANTO J., ESTALELLA R., TORRELLES J.M.
	Astrophys. J., 395, 494-500 (1992)
	Radio continuum from the powering sources of the RNO 43, HARO 4-255 FIR, B335, and PV Cephei outflows and from the Herbig-Haro object 32A.
o	Table 2: <[ARC92] LDN 1524 N> (Nos 1-3), <[ARC92] LDN 1527 N> (Nos 1-2), <[ARC92] RNO 43 N> (Nos 1-6), <[ARC92] Haro 4-255 FIR N> (Nos 1-2), <[ARC92] AS 353A N> (Nos 1-5), <[ARC92] Barn 335 N> (Nos 1-7), <[ARC92] PV Cep N> (Nos 1-2)
Ref:	=1998AJ....116.2953A
by	ANGLADA G. , VILLUENDAS E., ESTALELLA R., BELTRAN M.T., RODRIGUEZ L.F., TORRELLES J.M., CURIEL S.
	Astron. J., 116, 2953-2964 (1998)
	Spectral indices of centimeter continuum sources in star-forming regions: implications on the nature of the outflow exciting sources.
o	* SSV 61 = SSV LDN 1630 61. T.2: sources in RNO 43 = [ARC92] RNO 43 N.
o	Table 2: <[ARC92] AS 353A N> (Nos 6-8) added, <[ARC92] Barn 335 NN> (Nos 8-12) added. Table 2: <[AVE98] LDN 1641N N> (Nos 1-7), <[AVE98] Haro 4-255 N> (Nos 1-2), <[AVE98] HH 24-26 NN> (Nos 1-11), <[AVE98] LDN 1617 N> (Nos 1-8), <[AVE98] LDN 1251B N> (Nos 1-4), <[AVE98] LDN 1262 N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Arch
Arch	(Archeops experiment)
Write:	<<Arch GLLL.ll+BB.bb>>
N:	302
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	Archeops balloon-borne experiment by-product: catalog of bright smm point sources. See also [DMM2008].
Ref:	=2008A&A...481..411D
by	DESERT F.-X. , MACIAS-PEREZ J.F., MAYET F., GIARDINO G., RENAULT C., AUMONT J., BENOIT A., BERNARD J.-P., PONTHIEU N., TRISTRAM M.
	Astron. Astrophys., 481, 411-421 (2008)
	Submillimetre point sources from the Archeops experiment: very cold clumps in the Galactic plane.
o	Table 3, col(1): <[DMM2008] NNN> (Nos 1-302) = Table 3, col(2): <Arch GLLL.ll+BB.bb> N=302.
=E=	Catalogue in electronic form as J/A+A/481/411
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Ard
Ard	(?)
Write:	<<** Ard NNN>>
Object:	(SIMBAD class: = Double or Multiple Star)
Details on Acronym: [ARD2007]
[ARD2007]	(Adami+Russeil+Durret, 2007)
Write:	<<[ARD2007] JHHMMSS.s+DDMMSS.s>>
N:	14
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	OHP 120cm observations of RX J1119.7+2126. N=14 objects included in the central concentration.
Ref:	=2007A&A...467..459A
by	ADAMI C. , RUSSEIL D., DURRET F.
	Astron. Astrophys., 467, 459-463 (2007)
	The isolated fossil group RX J1119.7+2126.
o	Table 3: <[ARD2007] JHHMMSS.s+DDMMSS.s> N=14.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ardb
Ardb	(Ardeberg+)= (A) = Ardeberg = (C)
Write:	<<ARDB NNN>> <<ARDB CNN>>
N:	732
Object:	* (SIMBAD class: Star)
Note:	(Nos 1-409), LMC . (Nos 501-542), Possible LMC (Nos 601-732), Galactic * (Nos C1-C72):, newly defined stars. Identif. charts for the newly defined stars.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1972A&AS....6..249A
by	ARDEBERG A. , BRUNET J.P., MAURICE E., PREVOT L.
	Astron. Astrophys., Suppl. Ser., 6, 249-309 (1972)
	Spectrographic and photometric observations of supergiants and foreground stars, in the direction of the Large Magellanic Cloud.
o	Part 1, 2, 3: <ARDB NNN> (Nos 1-732), <ARDB CNN> (Nos C1-C61)
Ref:	=1973A&AS....9..447B
by	BRUNET J.P. , PREVOT L., MAURICE E., MURATORIO G.
	Astron. Astrophys., Suppl. Ser., 9, 447-458 (1973)
	Additional observations of supergiants and foreground stars in the direction of the Large Magellanic Cloud.
o	<ARDB CNN> (Nos C62-C72)
Details on Acronym: Ardeberg
Ardeberg	(Ardeberg+)
*****	Avoid the usage of Ardeberg, prefer Ardb
Details on Acronym: [ARF2020]
[ARF2020]	(Alabi+Romanowsky+Forbes+, 2020)
Write:	<<[ARF2020] COMA NN NNNN>> <<[ARF2020] COMA_NN_NNNN>> (not recognised by Simbad, but found in literature)
N:	9179
Object:	LSB (SIMBAD class: LowSurfBrghtG = Low Surface Brightness Galaxy)
Note:	Subaru Suprime-Cam osbervations of N=9174 galaxies in the direction of the Coma cluster. In format, COMA NN (10≤NN≤43) refers to the data sets from Okabe et al. 2014ApJ...784...90O.
in source:	ACO 1656 = Coma Cluster
Ref:	=2020MNRAS.496.3182A
by	ALABI A.B. , ROMANOWSKY A.J., FORBES D.A., BRODIE J.P., OKABE N.
	Mon. Not. R. Astron. Soc., 496, 3182-3197 (2020)
	An expanded catalogue of low surface brightness galaxies in the Coma cluster using Subaru/Suprime-Cam.
o	Tables 2-3: <[ARF2020] COMA NN NNNN> N=9174.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ARG
ARG	(Not yet in Simbad)
*****	Avoid the usage of ARG, prefer [G74]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: ARG
ARG	(Argelander)
Write:	<<** ARG NN>>
N:	99
Object:	(SIMBAD class: = Double or Multiple Star)
Details on Acronym: [ARG94]
[ARG94]	(Anglada+Rodriguez+Girart+, 1994)= (VLA)
Write:	<<[ARG94] VLA N>>
N:	5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA sources in LDN 1287.
in source:	LDN 1287
Ref:	=1994ApJ...420L..91A
by	ANGLADA G. , RODRIGUEZ L.F., GIRART J.M., ESTALELLA R., TORRELLES J.M.
	Astrophys. J., 420, 91-93 (1994)
	A radio candidate for the exciting source of the L 1287 bipolar outflow.
o	Table 1: <[ARG94] VLA N> N=4
Ref:	=2002RMxAA..38..161R
by	RODRIGUEZ M. , RODRIGUEZ L.F., GYULBUDAGHIAN A.L., MAY J.
	Rev. Mex. Astron. Astrofis., 38, 161-167 (2002)
	VLA detection of the exciting sources of the HH 288 and HHL 59 outflows.
o	Table 2: <[ARG94] VLA N> (No. 5) added. Table 2: <[RRG2002] HH 288 VLA N> (Nos 1-3), <[RRG2002] HHL 59 VLA N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ARGO
ARGO	(Astrophysical Radiation with Ground-based Observatory)
Write:	<<ARGO JHHMM+DDMM>>
N:	11
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	The Astrophysical Radiation with Ground-based Observatory at Yang Ba Jing (ARGO-YBJ) observations of N=11 gamma-ray sources.
Ref:	=2013ApJ...779...27B
by	BARTOLI B. , BERNARDINI P., BI X.J., BOLOGNINO I., BRANCHINI P., BUDANO A., CALABRESE MELCARNE A.K., CAMARRI P., CAO Z., CARDARELLI R., CATALANOTTI S., CHEN S.Z., CHEN T.L., CHEN Y., CRETI P., CUI S.W., DAI B.Z., D'AMONE A., DANZENGLUOBU, DE MITRI I., D'ETTORRE PIAZZOLI B., DI GIROLAMO T., DING X.H., DI SCIASCIO G., FENG C.F., FENG Z., FENG Z., GOU Q.B., GUO Y.Q., HE H.H., HU H., HU H., HUANG Q., IACOVACCI M., IUPPA R., JIA H.Y., LABACIREN, LI H.J., LI J.Y., LI X.X., LIGUORI G., LIU C., LIU C.Q., LIU J., LIU M.Y., LU H., MA L.L., MA X.H., MANCARELLA G., MARI S.M., MARSELLA G., MARTELLO D., MASTROIANNI S., MONTINI P., NING C.C., PANAREO M., PANICO B., PERRONE L., PISTILLI P., RUGGIERI F., SALVINI P., SANTONICO R., SBANO S.N., SHEN P.R., SHENG X.D., SHI F., SURDO A., TAN Y.H., VALLANIA P., VERNETTO S., VIGORITO C., WANG B., WANG H., WU C.Y., WU H.R., XU B., XUE L., YANG Q.Y., YANG X.C., YAO Z.G., YUAN A.F., ZHA M., ZHANG H.M., ZHANG J., ZHANG J., ZHANG L., ZHANG P., ZHANG X.Y., ZHANG Y., ZHAO J., ZHAXICIREN, ZHAXISANGZHU, ZHOU X.X., ZHU F.R., ZHU Q.Q., ZIZZI G., (The ARGO-YBJ Collaboration)
	Astrophys. J., 779, 27 (2013)
	TeV γ-ray survey of the northern sky using the ARGO-YBJ detector.
o	Table 2: <ARGO JHHMM+DDMM> N=11.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Argue
Argue	(Argue) (Not yet in Simbad)
*****	Avoid the usage of Argue, prefer [A63]
Origin	of the Acronym: L (2008A&A...491..951M)
Details on Acronym: Ariel
Ariel	(Ariel satellite)
*****	Avoid the usage of Ariel, prefer 1A
Details on Acronym: Ariel
Ariel	(Ariel satellite)
*****	Avoid the usage of Ariel, prefer 2A
Details on Acronym: Ariel
Ariel	(Ariel satellite)
*****	Avoid the usage of Ariel, prefer 3A
Details on Acronym: Ark
Ark	(Arakelian)= Akn = (Arak) = Arakelian = (Arakeljan) = (Arakelyan)
Write:	<<Ark NNN>>
N:	591
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Identif. charts
Ref:	=1975SoByu..47....3A
by	ARAKELIAN M.A.
	Soobshch. Byurakan Obs., 47, 3-40 (1975)
	The galaxies of high surface brightness.
o	Table 2: <Ark NNN> (Nos 1-591)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [ARK2001]
[ARK2001]	(Alonso-Herrero+Ryder+Knapen, 2001) (Not yet in Simbad)
Write:	<<[ARK2001] NN>> <<[ARK2001] HN>>
N:	18+8
Object:	Cluster of * + HII (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST NICMOS observations. Table 3, Fig.3: N=18 Cl* in NGC 2903. Table 4: N=8 HII regions in NGC 2903.
in source:	NGC 2903
Ref:	=2001MNRAS.322..757A
by	ALONSO-HERRERO A. , RYDER S.D., KNAPEN J.H.
	Mon. Not. R. Astron. Soc., 322, 757-769 (2001)
	Nuclear star formation in the hotspot galaxy NGC 2903.
o	Table 3, Fig.3: <[ARK2001] NN> (Nos 1-18). Table 4: <[ARK2001] HN> (Nos H1-H8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ARK2014]
[ARK2014]	(Atek+Richard+Kneib+, 2014)
Write:	<<[ARK2014] NNNNa>> <<[ARK2014] N.N>>
N:	29+13
Object:	G + Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST (ACS and WFC3) and Spitzer (IRAC) observations of the galaxy cluster Abell 2744, as part of the Hubble Frontier Fields program. N=15 I₈₁₄ dropout candidates at z∼6-7, N=1 Y₁₀₅ dropout at z∼8, and N=13 images of five multiply imaged systems were detected.
in source:	ACO 2744
Ref:	=2014ApJ...786...60A
by	ATEK H. , RICHARD J., KNEIB J.-P., CLEMENT B., EGAMI E., EBELING H., JAUZAC M., JULLO E., LAPORTE N., LIMOUSIN M., NATARAJAN P.
	Astrophys. J., 786, 60 (2014)
	Probing the z > 6 universe with the first Hubble frontier fields cluster A2744.
o	Fig. 3, Tables 2-3: <[ARK2014] NNNNa> N=15+1+13 among (Nos 93-3822). Fig. 3, Table 3: <[ARK2014] N.N> N=13 among (Nos 1.1-1.3 to 5.1-5.4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ARK2015]
[ARK2015]	(Atek+Richard+Kneib+, 2015)
Write:	<<[ARK2015] NNNN>> <<[ARK2015] N.N>>
N:	58+9
Object:	G + Grav. lensed image of a G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST (ACS and WFC3) observations of the galaxy cluster Abell 2744, as part of the Hubble Frontier Fields program. N=50 I₈₁₄ dropout candidates at z∼7, N=8 Y₁₀₅ dropout at z∼8, and N=9 images of three multiply imaged systems were detected.
in source:	ACO 2744
Ref:	=2015ApJ...800...18A
by	ATEK H. , RICHARD J., KNEIB J.-P., JAUZAC M., SCHAERER D., CLEMENT B., LIMOUSIN M., JULLO E., NATARAJAN P., EGAMI E., EBELING H.
	Astrophys. J., 800, 18 (2015)
	New constraints on the faint end of the UV luminosity function at z ~ 7-8 using the gravitational lensing of the Hubble frontier fields cluster A2744.
o	Tables 3-4: <[ARK2015] NNNN> N=50+8 among (Nos 260-6670). Table 5: <[ARK2015] N.N> (Nos 1.1-1.3, 2.1-2.2, 5.1-5.4).
=E=	Catalogue in electronic form as <J/ApJ/800/18/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ARK2016]
[ARK2016]	(Abreu-Vicente +Ragan+Kainulainen+, 2016)
Write:	<<[ARK2016] GMF NNN.N-NNN.Na>> <<[ARK2016] FLLL.l+BB.ba>> (not recognised by Simbad, but found in literature)
N:	12+10
Object:	Filament (SIMBAD class: ISM = Interstellar Medium Object)
Note:	N=10 giant molecular filaments (GMF) in the Milky Way. Use of archival Spitzer GLIMPSE, Herschel ATLASGAL, 2MASS, and Mopra ThrUMMS data. See also [RHT2014].
Ref:	=2016A&A...590A.131A
by	ABREU-VICENTE J. , RAGAN S., KAINULAINEN J., HENNING T., BEUTHER H., JOHNSTON K.
	Astron. Astrophys., 590A, 131-131 (2016)
	Giant molecular filaments in the Milky Way. II. The fourth Galactic quadrant.
o	G333 not identified.
o	Tables 2-3: <[ARK2016] GMF NNN.N-NN.Na> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ARK2020]
[ARK2020]	(Angioni+Ros+Kadler+, 2020)
Write:	<<[ARK2020] PS JHHMM.m+DDMM>>
N:	5
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	N=5 gamma-ray sources in the field of two 3FGL sources. Use of Fermi-LAT data.
Ref:	=2020A&A...641A.152A
by	ANGIONI R. , ROS E., KADLER M., OJHA R., MULLER C., EDWARDS P.G., BURD P.R., CARPENTER B., DUTKA M.S., GULYAEV S., HASE H., HORIUCHI S., KRAUSS F., LOVELL J.E.J., NATUSCH T., PHILLIPS C., PLOTZ C., QUICK J.F.H., ROSCH F., SCHULZ R., STEVENS J., TZIOUMIS A.K., WESTON S., WILMS J., ZENSUS J.A.
	Astron. Astrophys., 641A, 152-152 (2020)
	γ-ray emission in radio galaxies under the VLBI scope. II. The relationship between γ-ray emission and parsec-scale jets in radio galaxies.
o	Figs 9-10, Paragr. 3.3: <[ARK2020] PS JHHMM.m+DDMM> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ARL2002]
[ARL2002]	(Andreuzzi+Richer+Limongi+, 2002)
Write:	<<[ARL2002] NNNNNN>>
N:	223
Object:	* in Cl* (SIMBAD class: Star)
Note:	HST WFPC2 observations. Search for white dwarf in NGC 188. In the format 'NNNNNN', the first digit stands for the field 1 to 4, the second digit for the camera 2, 3, 4 (WF2, WF3, WF4).
in source:	NGC 188
Ref:	=2002A&A...390..961A
by	ANDREUZZI G. , RICHER H.B., LIMONGI M., BOLTE M.
	Astron. Astrophys., 390, 961-965 (2002)
	The white dwarf cooling sequence in the old open cluster NGC 188.
o	Catalog: <[ARL2002] NNNNNN> N=223.
=E=	Catalogue in electronic form as J/A+A/390/961
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ArM
ArM	(Ardeberg+Maurice)
*****	Avoid the usage of ArM, prefer [AM77]
Origin	of the Acronym: L (1982A&AS...50..291A)
Details on Acronym: Arm
Arm	(Arm feature)
Write:	<<NAME Arm W N in M 31>>
N:	7+7
Object:	Arm (SIMBAD class: PartofG = Part of a Galaxy)
Note:	In the format 'W N' stands for: 'N 1' to 'N 7' and 'S 1' to 'S 7' where N and S refer to arms on the North following and South preceding sides of the major axis. These arms were also studied by Baade in 1963 (Evolution of stars and galaxies).
in source:	M 31 = NGC 224
Ref:	=1964ApJ...139.1045A
by	ARP H.C.
	Astrophys. J., 139, 1045-1057 (1964)
	Spiral structure in M 31.
o	<NAME Arm W N in M 31> (Nos N 1 to N 7) and (Nos S 1 to S 7)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Arm
Arm	(Arm feature)
Write:	<<NAME Arm W R in M 33>>
N:	5+5
Object:	Arm (SIMBAD class: PartofG = Part of a Galaxy)
Note:	In the format 'W R' stands for: 'N I' to 'N V' and 'S I' to 'S V' where N and S refer to arms on the North following and South preceding sides of the major axis
in source:	M 33 = NGC 598
Ref:	=1980ApJ...236L...1S
by	SANDAGE A. , HUMPHREYS R.A.
	Astrophys. J., 236, 1-5 (1980)
	On the warped optical plane of M 33.
o	<NAME Arm W R in M 33> (Nos N I to N V) and (Nos S I to S V)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [ARM2000]
[ARM2000]	(Argon+Reid+Menten, 2000)
Write:	<<[ARM2000] GLLL.lll+BB.bbb>>
N:	91
Object:	OH Maser (SIMBAD class: Maser)
Note:	See also [BE83], Caswell OH and [CPF88].
Ref:	=2000ApJS..129..159A
by	ARGON A.L. , REID M.J., MENTEN K.M.
	Astrophys. J., Suppl. Ser., 129, 159-227 (2000)
	Interstellar hydroxyl masers in the galaxy. I. The VLA survey.
o	Table 1: <[ARM2000] GLLL.lll+BB.bbb> N=91.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ARM2016]
[ARM2016]	(Arellano-Cordova+Rodriguez+Mayya+, 2018)
Write:	<<[ARM2016] NN>>
N:	48
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	GTC Osiris observations of N=48 HII regions in the M81 galaxy.
in source:	M 81 = NGC 3031
Ref:	=2016MNRAS.455.2627A
by	ARELLANO-CORDOVA K.Z. , RODRIGUEZ M., MAYYA Y.D., ROSA-GONZALEZ D.
	Mon. Not. R. Astron. Soc., 455, 2627-2643 (2016)
	The oxygen abundance gradient in M81 and the robustness of abundance determinations in HII regions.
o	Table 2: <[ARM2016] NN> (Nos 1-48).
=E=	Catalogue in electronic form as J/MNRAS/455/2627
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ARM2018]
[ARM2018]	(Arrabal Haro+Rodriguez Espinosa+Munoz-Tunon+, 2018)
Write:	<<[ARM2018] SHARDSNNNNNNNN>>
N:	1558
Object:	G (SIMBAD class: Galaxy)
Note:	N=1558 sources in the SHARDS survey, in search for high-z galaxies.
Ref:	=2018MNRAS.478.3740A
by	ARRABAL HARO P. , RODRIGUEZ ESPINOSA J.M., MUNOZ-TUNON C., PEREZ-GONZALEZ P.G., DANNERBAUER H., BONGIOVANNI A., BARRO G., CAVA A., LUMBRERAS-CALLE A., HERNAN-CABALLERO A., ELICHE-MORAL M.C., DOMINGUEZ SANCHEZ H., CONSELICE C.J., TRESSE L., ALCALDE PAMPLIEGA B., BALCELLS M., DADDI E., RODIGHIERO G.
	Mon. Not. R. Astron. Soc., 478, 3740-3755 (2018)
	A simultaneous search for high-z LAEs and LBGs in the SHARDS survey.
o	Table 1: <[ARM2018] SHARDSNNNNNNNN> N=1558 among (Nos 10000066-20025450).
=E=	Catalogue in electronic form as <J/MNRAS/478/3740/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [ARM90]
[ARM90]	(Aspin+Rayner+McLean+, 1990)
Write:	<<[ARM90] R>>
N:	7
Object:	Region (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	UKIRT observations. Regions observed in J, H, K wavelengths in Sh 2-106 HII region.
in source:	SH 2-106
Ref:	=1990MNRAS.246..565A
by	ASPIN C. , RAYNER J.T., McLEAN I.S., HAYASHI S.S.
	Mon. Not. R. Astron. Soc., 246, 565-575 (1990)
	Infrared polarimetry and photometry of S 106.
o	Table 1: <[GGC82] IRS 3W> (No. 3N) added. Tables 1, 2, Fig.2: <[ARM90] R> (Nos I to VII).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ArMa
ArMa	(Ardeberg+Maurice)
*****	Avoid the usage of ArMa, prefer [AM77]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: ArMa
ArMa	(Ardeberg+Maurice)
Write:	<<ArMa NNN>>
N:	139
Object:	* (SIMBAD class: Star)
Note:	J.-C. Mermilliod has added (Nos 126-139), and cross-id. with 'Cl* IC 2944 THA NN' numbering. Same authors and same year in ref. 1977A&AS...30..261A: see [AM77].
in source:	IC 2944
Ref:	=1977A&AS...28..153A
by	ARDEBERG A. , MAURICE E.
	Astron. Astrophys., Suppl. Ser., 28, 153-168 (1977)
	A spectrographic and photometric study of stars and interstellar medium surrounding HD 101205.
o	Acronym ArMa used for this ref. in SIMBAD. Acronym [AM77] is used for ref. 1977A&AS...30..261A.
o	<ArMa NNN> (Nos 1-125)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: ARO
ARO	(Algonquin Radio Obs.) (Not yet in Simbad)
Write:	<<ARO HHMM+DD>>
N:	15
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Radio-sources with low frequency cut off, named 'ARO HHMM+DD' by ROSS H.N., in his Ph. D. Thesis, Univ. of Toronto, Canada, 1972. The thesis also contains 2 sources with NRAO number.
Auth.:	ROSS H.N.
Details on Acronym: ARO
ARO	(Algonquin Radio Obs.)
Write:	<<PN ARO NNN>>
N:	557
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Ref:	=1971PAB.....1....1H
by	HIGGS L.A.
	Publ. Astrophys. Branch, Nat. Research Council Canada, 1, 1-None (1971)
	Catalog of radio observations of planetary nebulae, related optical data.
o	<PN ARO NNN> (Nos 1-557).
Details on Acronym: Arp
Arp	(Arp)
====>	Equivalent to: APG
Details on Acronym: Arp
Arp	(Arp)
Write:	<<Cl Arp N>>
N:	2
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Ref:	=1960PASP...72...48A
by	ARP H. , VAN DEN BERGH S.
	Publ. Astron. Soc. Pac., 72, 48-51 (1960)
	A new faint globular cluster.
o	<Cl Arp N> (Nos 1-2)
Details on Acronym: ARS
ARS	(Autofib Redshift Survey)
Write:	<<ARS BHHMMSS.ss+DDMMSS.s>>
N:	2522
Object:	* + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	In preparation. These (unpublished) data are discussed 1997MNRAS.285..613H, Autofib Redshift Survey - II. Evolution of the galaxy luminosity function by spectral type, by Jeremy Heyl, Matthew Colless, Richard S. Ellis and Tom Broadhurst. Objects are individually unpublished, but collectively described in 1997MNRAS.285..613H and 1994MNRAS.267..541C. They have been donated to NED. The data are distributed in tabular form without a formal name attached. The names have been created strictly by taking the acronym and prepending it to the listed coords. Thus, no rounding or truncating has been performed. It may be overkill, but it does uniquely identify the objects.
Auth.:	SCHMITZ M.+ IPAC
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: Art
Art	(Artyukhina)
*****	Avoid the usage of Art, prefer Arty
Origin	of the Acronym: L (2008A&A...491..951M)
Details on Acronym: Arty
Arty	(Artyukhina)= (Art)
Write:	<<Arty NNNN>>
N:	2070
Object:	* (SIMBAD class: Star)
Note:	J.-C. Mermilliod has added (Nos 1074-2070)
in source:	NAME NGP
Ref:	=1955TrSht..26....3A
by	ARTYUKHINA N.M.
	Trudy Gosud. Astron. Inst. Shternberga, 26, 3-123 (1955)
	Definition et analyse d'etoiles a mouvement propre dans la region du pole Nord galactique. (en russe).
o	<Arty NNNN> N=1073
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ARV2008]
[ARV2008]	(Antokhin+Rauw+Vreux+, 2008)
Write:	<<[ARV2008] NNN>>
N:	235
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton study of Car OB 1 association.
in source:	NAME ASS CAR OB 1-
Ref:	=2008A&A...477..593A
by	ANTOKHIN I.I. , RAUW G., VREUX J.-M., VAN DER HUCHT K.A., BROWN J.C.
	Astron. Astrophys., 477, 593-609 (2008)
	XMM-Newton X-ray study of early type stars in the Carina OB1 association.
o	Tables 2, 3: <[ARV2008] NNN> (Nos 1-235).
=E=	Catalogue in electronic form as <J/A=A/477/593>
=E=	Catalogue in electronic form as <J/A+A/477/593/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ARX2000]
[ARX2000]	(Alton+Rand+Xilouris+, 2000) (Not yet in Simbad)
Write:	<<[ARX2000] NGC 891 A>>
N:	4
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Note:	N=4 features in NGC 891. A and B are chimney-like structures, C and D are isolated dust clouds.
in source:	NGC 891
Ref:	=2000A&AS..145...83A
by	ALTON P.B. , RAND R.J., XILOURIS E.M., BEVAN S., FERGUSON A.M., DAVIES J.I., BIANCHI S.
	Astron. Astrophys., Suppl. Ser., 145, 83-109 (2000)
	Dust outflows from quiescent spiral disks.
o	Fig.1, Table 5: <[ARX2000] NGC 891 A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ARXA
ARXA	(Atlas of Radio/X-ray Associations)
Write:	<<ARXA JHHMMSS.s+DDMMSS>>
N:	602570
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	All-sky comprehensive catalogue of calculated radio and X-ray associations to optical objects.
Ref:	=2010PASA...27..283F
by	FLESCH E.
	PASA, 27, 283-289 (2010)
	An All-Sky Atlas of Radio/X-ray Associations.
o	Table 7: <ARXA JHHMMSS.s+DDMMSS> N=602570.
=E=	Catalogue in electronic form as V/134
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: As
As	(Asiago obs.)
Object:	V* (SIMBAD class: Variable* = Variable Star)
Rem:	V* Nomenclature.
Details on Acronym: AS
AS	(Aspin Source?)
*****	Avoid the usage of AS, prefer [A98b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AS
AS	(Additional Star)
Write:	<<*Em AS** NNNA>>
N:	521
Object:	Em* + PN (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Note:	Continues MWC. N=521 among which 39 PN.
Ref:	=1950ApJ...112...72M
by	MERRILL P.W. , BURWELL C.G.
	Astrophys. J., 112, 72-89 (1950)
	Additional stars whose spectra have a bright H-α line.
o	Table I: <Em* AS NNN> (Nos 1-519)
Ref:	=1951ApJ...113..624M
by	MILLER W.C. , MERRILL P.W.
	Astrophys. J., 113, 624-625 (1951)
	Spectroscopic observations of Be stars.
o	Table 1: <Em* AS NNN> (Nos 520-521)
Details on Acronym: AS
AS	(ARNICA Standard)
*****	Avoid the usage of AS, prefer [HMT98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: As
As	(Assoc.)
*****	Avoid the usage of As, prefer [PGF2001]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AS
AS	(Association)
*****	Avoid the usage of AS, prefer [PUG2005]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AS2012]
[AS2012]	(Alis+Saygac, 2012)
Write:	<<[AS2012] NNNNN>>
N:	4+29
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	HST WFPC2 archival observations of N=4 novae and N=29 other variable stars in NGC 3627.
in source:	NGC 3627
Ref:	=2012NewA...17..101A
by	ALIS S. , SAYGAC A.T.
	NewA, 17, 101-107 (2012)
	Archival HST study of novae. I. The Seyfert galaxy NGC 3627.
o	Tables 2, 4, 5: <[AS2012] NNNNN> N=4+29 among (Nos 953-12587).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AS2019]
[AS2019]	(Agnello+Spiniello, 2019)
Write:	<<[AS2019] WG J210014.9-445206.4>> <<[AS2019] WG J021416.37-210535.3>> <<[AS2019] JHHMMSS.ss+DDMMSS.s>> <<[AS2019] WG 210014.9-445206.4>> (not recognised by Simbad, but found in literature) <<[AS2019] WG 021416.37-210535.3>>
N:	1+1+97
Object:	Poss. Grav. lensed image of a QSO (SIMBAD class: LensedImage_Candidate = Gravitationally Lensed Image Candidate)
Note:	N=2+97 gravitationally lensed images of quasars in the Dark Energy Survey DR1 footprint. Use of DES DR1, Gaia DR1 and DR2, and WISE data.
Ref:	=2019MNRAS.489.2525A
by	AGNELLO A. , SPINIELLO C.
	Mon. Not. R. Astron. Soc., 489, 2525-2535 (2019)
	Quasar lenses in the south: searches over the DES public footprint.
o	<[AS2019] WG J210014.9-445206.4> N=1. <[AS2019] WG J021416.37-210535.3> N=1. Tables A1-A2: <[AS2019] JHHMMSS.ss+DDMMSS.s> N=97.
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: AS2COS
AS2COS	(ALMA-S2COSMOS)
Write:	<<AS2COS NNNN.N>>
N:	260
Object:	smm G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 7 (0.87mm) observations of N=260 sub-millimetre galaxies, as part of the ALMA-S2COSMOS (AS2COSMOS) pilot survey. Use of S2COSMOS data.
in source:	NAME COSMOS Field
Ref:	=2020MNRAS.495.3409S
by	SIMPSON J.M. , SMAIL I., DUDZEVICIUTE U., MATSUDA Y., HSIEH B.-C., WANG W.-H., SWINBANK A.M., STACH S.M., AN F.X., BIRKIN J.E., AO Y., BUNKER A.J., CHAPMAN S.C., CHEN C.-C., COPPIN K.E.K., IKARASHI S., IVISON R.J., MITSUHASHI I., SAITO T., UMEHATA H., WANG R., ZHAO Y.
	Mon. Not. R. Astron. Soc., 495, 3409-3430 (2020)
	An ALMA survey of the brightest sub-millimetre sources in the SCUBA-2-COSMOS field.
o	Table 1: <AS2COSNNNN.N> N=260 among (Nos 0001.1-0426.1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AS2UDS
AS2UDS	(ALMA-SCUBA-2 survey of the Ultra Deep Survey field)
Write:	<<AS2UDS NNNN.N>> <<AS2UDS JHHMMSS.ss+DDMMSS.ss>>
N:	708*2
Object:	smm G (SIMBAD class: Galaxy)
Note:	ALMA Band 7 continuum observations of N=708 sub-millimetre galaxies (SMGs) in the UKIDSS/UDS field, selected from the SCUBA-2 Cosmology Legacy Survey (S2CLS). In format NNN.N: "NNNN" is the source identifier from the parent S2CLS survey and the final digit identifies the individual galaxies detected with ALMA in the S2CLS source with ascending numbers for descending flux.
Ref:	=2019MNRAS.487.4648S
by	STACH S.M. , DUDZEVICIUTE U., SMAIL I., SWINBANK A.M., GEACH J.E., SIMPSON J.M., AN F.X., ALMAINI O., ARUMUGAM V., BLAIN A.W., CHAPMAN S.C., CHEN C.-C., CONSELICE C.J., COOKE E.A., COPPIN K.E.K., DA CUNHA E., DUNLOP J.S., FARRAH D., GULLBERG B., HODGE J.A., IVISON R.J., KOCEVSKI D.D., MICHALOWSKI M.J., MIYAJI T., SCOTT D., THOMSON A.P., WARDLOW J.L., WEISS A., VAN DER WERF P.
	Mon. Not. R. Astron. Soc., 487, 4648-4668 (2019)
	An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: source catalogue and properties.
o	<AS2UDS NNNN.N> N=708 among (Nos 0001.0-0001.1 to 0812.0) = <AS2UDS JHHMMSS.ss+DDMMSS.ss> N=708.
=E=	Catalogue in electronic form as <J/MNRAS/487/4648/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AS58]
[AS58]	(Ambartsumian+Schachbazian, 1958)= (ASh) (Not yet in Simbad)
Write:	<<[AS58] NN>>
N:	10
Object:	Blue Obj. (SIMBAD class: blue = Blue Object)
Ref:	=1958DoArm..26..277A
by	AMBARTSUMIAN V.A. , SCHACHBAZIAN R.K.
	Doklady - Akad. Nauk Arm. SSR, 26, 277-279 (1958)
	Galaxies multiples et radio-galaxies. IV. Objets bleus proches et galaxies elliptiques.
o	<[AS58] NN> (Nos 1-10).
Details on Acronym: [AS79]
[AS79]	(Arp+Sulentic, 1979)= (BSO) = (RSO)
Write:	<<[AS79] NGC 1073 BSO N>> <<[AS79] NGC 1073 RSO>>
N:	2+1
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	In the vicinity of NGC 1073
Ref:	=1979ApJ...229..496A
by	ARP H. , SULENTIC J.W.
	Astrophys. J., 229, 496-502 (1979)
	Three quasars near the spiral arms of NGC 1073.
o	<[AS79] NGC 1073 BSO N> (Nos 1-2), <[AS79] NGC 1073 RSO> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AS82]
[AS82]	(Arp+Surdej, 1982)= ([AS82a])
Write:	<<[AS82] A>> <<[AS82] NNN>>
N:	25+137
Object:	* + QSO + (UV) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 1: (Nos A-Y), N=13 stars, + N=12 QSO, named 'CF 1549+48A' in the Veron catalogue of QSO Fig.1a: (Nos 1-137) UV candidates, No. 46 is named 'CF 1549+48 6' in the Veron catalogue of QSO.
Ref:	=1982A&A...109..101A
by	ARP H. , SURDEJ J.
	Astron. Astrophys., 109, 101-106 (1982)
	Quasars in a control field far from bright galaxies.
o	In 'Veron and Veron' QSO catalogue: [AS82] A = CF 1549+48A, [AS82] 46 = CF 1549+48#46
o	Table 1: <[AS82] A> (Nos A-Y). Fig.1a: <[AS82] NNN> (Nos 1-137)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AS82a]
[AS82a]	(Arp+Surdej, 1982)
*****	Avoid the usage of [AS82a], prefer [AS82]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AS82b]
[AS82b]	(Andronov+Shugarov, 1982)
Write:	<<[AS82b] a>> <<[AS82b] NN>>
N:	12+20
Object:	Comparison * (SIMBAD class: Star)
Ref:	=1982ATsir1218....3A
by	ANDRONOV I.L. , SHUGAROV S.Y.
	Astron. Tsirk., 1218, 3-5 (1982)
	A photometric study of MV Lyrae.
o	Table, Fig.: <[AS82b] a> N=10 among (Nos b-m), <[AS82b] N> (Nos 1-9).
Ref:	=1993PASP..105...51R
by	ROSINO L. , ROMANO G., MARZIANI P.
	Publ. Astron. Soc. Pac., 105, 51-58 (1993)
	Photometric and spectroscopic observations of MV Lyrae from from 1968 to 1991.
o	Table 1: <[AS82b] a> (Nos o, p) added.
Ref:	=1998ARep...42..370S
by	SHUGAROV S.Y. , PAVLENKO E.P.
	Astron. Rep., 42, 370-376 (1998)
	MV Lyr in low brightness states: outbursts.
o	Table 1: <[AS82b] NN> (Nos 11-22) added, Nos 10 and 18 missing.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AS99]
[AS99]	(Abolmasov+Shugarov, 1999) (Not yet in Simbad)
Write:	<<[AS99] a>>
N:	10
Object:	* (SIMBAD class: Star)
Note:	Fig.1: Finding chart of IRAS 17506+3411 with N=10 comparison stars (Nos a-j).
Ref:	=1999IBVS.4735....1A
by	ABOLMASOV P.K. , SHUGAROV S.Y.
	IAU Inform. Bull. Var. Stars, 4735, 1-2 (1999)
	Discovery of a new Mira variable.
o	Fig.1: <[AS99] a> (Nos a-j).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ASA2011]
[ASA2011]	(Andjelic+Stavrev+Arbutina+, 2011)
Write:	<<[ASA2011] aNN>>
N:	12
Object:	Poss. HII (SIMBAD class: EmObj = Emission Object)
Stat:	is completely incorporated in Simbad
Note:	Rozhen observatory 2m RCC telescope observation of N=12 possible HII regions in the HI tidal arm ("Garland") near NGC 3077.
in source:	NAME Garland
Ref:	=2011BaltA..20..459A
by	ANDJELIC M. , STAVREV K., ARBUTINA B., ILIC D., UROSEVIC D.
	BaltA, 20, 459-462 (2011)
	Observations of the galaxy NGC 3077 in the narrow-band [SII] and H-α filters.
o	Fig. 1, Table 3: <[ASA2011] aNN> (Nos a1-a12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ASAGAO
ASAGAO	(ALMA twenty-Six Arcmin2 survey of GOODS-S at One mm)
*****	Avoid the usage of ASAGAO, prefer [FOK2018]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ASAGAO
ASAGAO	(ALMA twenty-Six Arcmin2 survey of GOODS-S at One mm)
*****	Avoid the usage of ASAGAO, prefer [HKY2018]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ASAS
ASAS	(All Sky Automated Survey)
Write:	<<ASAS JHHMMSS+DDMM.m>>
N:	126+106+132+3126+11357+10453+10311+11509
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	All Sky Automated Survey: for more information, visit http://www.astrouw.edu.pl/asas/ Only the first references with ASAS objects are listed here.
Ref:	=1998AcA....48...35P
by	POJMANSKI G.
	Acta Astron., 48, 35-58 (1998)
	The All Sky Automated Survey. The catalog of the periodic variable stars in the selected fields.
o	T.1 : Fields not in SIMBAD. T.3, rows 9 and 10 of the right column, OtherID are inverted. (Grzegorz Pojmanski, 14 Jan 1999)
o	Table 2: <ASAS JHHMMSS+DDMM.m> N=126
Ref:	=2000AcA....50..177P
by	POJMANSKI G.
	Acta Astron., 50, 177-190 (2000)
	The All Sky Automated Survey. Catalog of about 3800 variable stars.
o	Tables 3-4: <ASAS JHHMMSS+DDMM.m> N=106+132.
Ref:	=2002AcA....52..397P
by	POJMANSKI G.
	Acta Astron., 52, 397-427 (2002)
	The All Sky Automated Survey. Catalog of variable stars. I. 0h -6h quarter of the Southern hemisphere.
o	<ASAS JHHMMSS+DDMM.m> N=3126.
Ref:	=2003AcA....53..341P
by	POJMANSKI G.
	Acta Astron., 53, 341-369 (2003)
	The All Sky Automated Survey. The catalog of variable stars. II. 6h -12h quarter of the Southern Hemisphere.
o	Data taken from VizieR On-line Data Catalog: II/264.
o	Table 2: <ASAS JHHMMSS+DDMM.m> N=11357.
Ref:	=2004AcA....54..153P
by	POJMANSKI G. , MACIEJEWSKI G.
	Acta Astron., 54, 153-179 (2004)
	The All Sky Automated Survey. Catalog of variable stars. III. 12h -18h quarter of the southern hemisphere.
o	Data taken from VizieR On-line Data Catalog: II/264.
o	Table 2: <ASAS JHHMMSS+DDMM.m> N=10453.
Ref:	=2005AcA....55...97P
by	POJMANSKI G. , MACIEJEWSKI G.
	Acta Astron., 55, 97-122 (2005)
	The All Sky Automated Survey. Catalog of variable stars. IV. 18h-24h quarter of the southern hemisphere.
o	Data taken from VizieR On-line Data Catalog: II/264.
o	Table 2: <ASAS JHHMMSS+DDMM.m> N=10311.
Ref:	=2005AcA....55..275P
by	POJMANSKI G. , PILECKI B., SZCZYGIEL D.
	Acta Astron., 55, 275-301 (2005)
	The All Sky Automated Survey. Catalog of variable stars. V. Declinations 0 ° - +28 ° of the northern hemisphere.
o	Data taken from VizieR On-line Data Catalog: II/264.
o	<ASAS JHHMMSS+DDMM.m> N=11509.
=E=	Catalogue in electronic form as J/AcA/48/35
=E=	Catalogue in electronic form as J/AcA/50/177
=E=	Catalogue in electronic form as II/264
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ASASSN
ASASSN	(All-Sky Automated Survey for Supernovae)
Write:	<<ASASSN -YYaaa>>
N:	>500
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	The "All-Sky Automated Survey for Supernovae" (ASAS-SN or "Assassin") is a long-term project to monitor the whole sky with a 2-3 day cadence using a global network of telescopes with a modular design of commercially available telephoto lenses and CCDs. The focus of the survey is to find nearby supernovae (SNe) and other transient sources. ASAS-SN carries out a full-sky, fast cadence, bright, relatively low-cost survey. ASAS-SN finds and characterizes the closest and brightest transients, and these are the transients that are most easily studied in detail in order to understand their astrophysical properties. http://www.astronomy.ohio-state.edu/~assassin/index.shtml
Notes:	ASAS-SN is currently the leading discoverer of Supernovae brighter than 17th magnitude. (please see: http://www.rochesterastronomy.org/supernova.html) A list of our transients can be found here: http://www.astronomy.ohio-state.edu/~assassin/transients.html
Auth.:	Benjamin Shappee Carnegie Observatories
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: ASASSN-V
ASASSN-V	(ASAS-SN Catalog of Variable Stars)
Write:	<<ASASSN-V JHHMMSS.ss+DDMMSS.s>>
N:	66179
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Catalogue of N=66179 bright variable stars, compiled using observations taken by the "Brutus" (Haleakala, Hawaii) and "Cassius" (CTIO, Chile) quadruple telescopes between 2013 and 2017. The ASAS-SN variable stars database is available at: https://asas-sn.osu.edu/variables
Ref:	=2018MNRAS.477.3145J
by	JAYASINGHE T. , KOCHANEK C.S., STANEK K.Z., SHAPPEE B.J., HOLOIEN T.W.-S., THOMPSON T.A., PRIETO J.L., DONG S., PAWLAK M., SHIELDS J.V., POJMANSKI G., OTERO S., BRITT C.A., WILL D.
	Mon. Not. R. Astron. Soc., 477, 3145-3163 (2018)
	The ASAS-SN catalogue of variable stars I: The Serendipitous Survey.
o	The resolution of the ASAS-SN survey is 15''. As a consequence the astrometry is poor, usually within 5'', but it can be more than 1 pixel. Status of the catalogue II/366 in SIMBAD : Classical Cepheids (Type = DCEP or DCEPS, N=2183), and Mira Variables (Type = M, N=10230), have been enterely ingested; other LPVs are being processed. Objects with an undefined variability type (Type = VAR, N=62577) will not be ingested.
o	<ASASSN-V JHHMMSS.ss+DDMMSS.s> N=66179.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ASB
ASB	(A.S. Bennett)
Write:	<<ASB NN>>
N:	79
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1963MNRAS.127....3B
by	BENNETT A.S.
	Mon. Not. R. Astron. Soc., 127, 3-13 (1963)
	A survey of extended sources of radio emission.
o	Table I: <ASB NN> (Nos 1-79).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [ASB2009]
[ASB2009]	(Ashby+Stern+Brodwin+, 2009)
Write:	<<[ASB2009] SDWFS N.N DDD.ddddddd+DD.ddddddd>> <<[ASB2009] JHHMMSS.s+DDMMSS>>
N:	?+4
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Spitzer IRAC observations of the NDWF Bootes field. See also SDWFS.
in source:	NAME Bootes Field
Ref:	=2009ApJ...701..428A
by	ASHBY M.L.N. , STERN D., BRODWIN M., GRIFFITH R., EISENHARDT P., KOZLOWSKI S., KOCHANEK C.S., BOCK J.J., BORYS C., BRAND K., BROWN M.J.I., COOL R., COORAY A., CROFT S., DEY A., EISENSTEIN D., GONZALEZ A.H., GORJIAN V., GROGIN N.A., IVISON R.J., JACOB J., JANNUZI B.T., MAINZER A., MOUSTAKAS L.A., ROTTGERING H.J.A., SEYMOUR N., SMITH H.A., STANFORD S.A., STAUFFER J.R., SULLIVAN I., VAN BREUGEL W., WILLNER S.P., WRIGHT E.L.
	Astrophys. J., 701, 428-453 (2009)
	The Spitzer Deep, Wide-Field Survey.
o	Tables 6-9: <[ASB2009] SDWFS N.N DDD.ddddddd+DD.ddddddd> N=-. Table 26: <[ASB2009] JHHMMSS.s+DDMMSS> N=4.
=E=	Catalogue in electronic form as <J/ApJ/701/428/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ASC2008]
[ASC2008]	(Alcala Spezzi+Chapman+, 2008)
Write:	<<[ASC2008] NN>>
N:	63
Object:	PMS* + Poss. PMS* (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Stat:	is completely incorporated in Simbad
Note:	Spitzer c2d survey of the Cha II cloud complex to search for PMS stars.
in source:	NAME Cha II
Ref:	=2008ApJ...676..427A
by	ALCALA J.M. , SPEZZI L., CHAPMAN N., EVANS II N.J., HUARD T.L., JORGENSEN J.K., MERIN B., STAPELFELDT K.R., COVINO E., FRASCA A., GANDOLFI D., OLIVEIRA I.
	Astrophys. J., 676, 427-463 (2008)
	The Spitzer c2d survey of large, nearby, interstellar clouds. X. The Chamaeleon II Pre-Main-Sequence population as observed with IRAC and MIPS.
o	IRAS F12514-7641 misprint for IRAS F12514-7631, CHIIXR 60 misprint for ??
o	Table 1: <[ASC2008] NN> (Nos 1-63).
=E=	Catalogue in electronic form as J/ApJ/676/427
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ASC2017]
[ASC2017]	(Angelo+Santos+Corradi+, 2017)
Write:	<<[ASC2017] NN>>
N:	53
Object:	* (SIMBAD class: Star)
Note:	Gemini GMOS spectroscopic observations of N=53 stars in the NGC 7193 open cluster.
in source:	NGC 7193
Ref:	=2017RAA....17....4A
by	ANGELO M.S. , SANTOS J.F.C.Jr, CORRADI W.J.B., MAIA F.F.S., PIATTI A.E.
	RAA, 17, 4 (2017)
	Investigation of Galactic open cluster remnants: the case of NGC 7193.
o	Table 2: <[ASC2017] NN> N=53 among (Nos 2-62).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ASC2019]
[ASC2019]	(Artkop+Smith+Corsi+, 2019)
Write:	<<[ASC2019] VN>> <<[ASC2019] SNN>>
N:	7+25
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA VLITE 338MHz and VLA 1.4GHz observations of N=7+25 radio sources, as possible radio counterparts associated with the Fermi LAT candidate in the GrW 170608 error region.
Ref:	=2019ApJ...884...16A
by	ARTKOP K. , SMITH R., CORSI A., GIACINTUCCI S., PETERS W.M., PERNA R., CENKO S.B., CLARKE T.E.
	Astrophys. J., 884, 16-16 (2019)
	Radio follow-up of a candidate γ-ray transient in the sky localization area of GW170608.
o	Table 2: <[ASC2019] VN> (Nos V1-V7). Table 3: <[ASC2019] SNN> (Nos S1-S25).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ASCC
ASCC	(All-Sky Compiled Catalogue, 2500000 stars)= (ASCC-2.5)
Write:	<<ASCC NNNNNNN>>
N:	2501313
Object:	* (SIMBAD class: Star)
Note:	Catalogue of 2.5 million stars with the limiting magnitude V-12-14. Stars are numbered from 1 to 2501977 (as in the first version), and from 2600001 to 2603318 (new stars in the 2nd version). See also CRVAD and CSOCA.
Ref:	=2001KFNT...17e.409K
by	KHARCHENKO N.V.
	Kinematika Fiz. Nebesn. Tel., 17, part no 5, 409-None (2001)
	All-sky Compiled Catalogue of 2.5 million stars (ASCC-2.5).
o	Catalogue: <ASCC NNNNNNN> N=2501313 among (Nos 1-2603318).
=E=	Catalogue in electronic form as I/280
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ASCC
ASCC	(All-Sky Compiled Catalogue)
*****	Avoid the usage of ASCC, prefer [KPR2005]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ASCC-2.5
ASCC-2.5	(All-Sky Compiled Catalogue, 2500000 stars) (Not yet in Simbad)
*****	Avoid the usage of ASCC-2.5, prefer ASCC
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ASD2005]
[ASD2005]	(Adami+Slezak+Durret+, 2005)
Write:	<<[ASD2005] N>>
N:	4
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Images of the Coma Cluster in the B, V, R, I bands with the CFH12K camera at CFHT. Sources of diffuse emission are present in the central zone around the central galaxies NGC 4874 and NGC 4889.
in source:	Coma Cluster = ACO 1656
Ref:	=2005A&A...429...39A
by	ADAMI C. , SLEZAK E., DURRET F., CONSELICE C.J., CUILLANDRE J.-C., GALLAGHER J.S., MAZURE A., PELLO R., PICAT J.P., ULMER M.P.
	Astron. Astrophys., 429, 39-48 (2005)
	Large scale diffuse light in the Coma cluster: A multi-scale approach.
o	Table 1: <[ASD2005] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ASD79]
[ASD79]	(Arp+Sulentic+Di Tullio, 1979)= (U) = (UB)
Write:	<<[ASD79] NGC 3384 UBNN>> <<[ASD79] Gal 1>>
N:	16
Object:	UV Obj. + QSO (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	Plate 13: N=16 Ultraviolet excess objects format 'NGC 3384 UBNN' in the vicinity of the triple system of galaxies NGC 3379/84/89 Table 1: 8 are quasars (Nos UB1, UB2, UB4, UB5, UB8, UB13-UB15). Table 3: One galaxy, '[ASD79] Gal 1'
Ref:	=1979ApJ...229..489A
by	ARP H. , SULENTIC J.W., DI TULLIO G.
	Astrophys. J., 229, 489-495 (1979)
	Quasars aligned across NGC 3384.
o	Table 1, Pl.13: <[ASD79] NGC 3384 UBNN> (Nos UB1-UB16). Table 3: <[ASD79] Gal 1>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 1ASE
1ASE	(American Science and Engeneering) (Not yet in Simbad)
Write:	<<1ASE HHMM+DD>>
N:	16
Object:	(X) (SIMBAD class: X = X-ray Source)
Details on Acronym: 2ASE
2ASE	(American Science and Engeneering) (Not yet in Simbad)
Write:	<<2ASE HHMM+DD>>
N:	16
Object:	(X) (SIMBAD class: X = X-ray Source)
Details on Acronym: [ASF2023]
[ASF2023]	(Atek+Shuntov+Furtak+, 2023)
Write:	<<[ASF2023] SMACS z1Na>> <<[ASF2023] SMACS_z1Na>> (not recognised by Simbad, but found in literature)
N:	10
Object:	Poss. G (SIMBAD class: Galaxy_Candidate = Galaxy Candidate)
Note:	N=6+2+2 galaxy candidates in the field of the galaxy cluster SMACS J0723.3-7327, at z∼9-11, z∼12, and z∼16 respectively. Use of JWST NIRCam and NIRISS archival data.
in source:	SMACS J0723.3-7327
Ref:	=2023MNRAS.519.1201A
by	ATEK H. , SHUNTOV M., FURTAK L.J., RICHARD J., KNEIB J.-P., MAHLER G., ZITRIN A., McCRACKEN H.J., CHARLOT S., CHEVALLARD J., CHEMERYNSKA I.
	Mon. Not. R. Astron. Soc., 519, 1201-1220 (2023)
	Revealing galaxy candidates out to z ~ 16 with JWST observations of the lensing cluster SMACS0723.
o	Table 2: <[ASF2023] SMACS zNNa> (Nos z10a-z10e, z11a, Z12a-z12b, z16a-z16b).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [ASG2012]
[ASG2012]	(Adamo+Smith+Gallagher+, 2012) (Not yet in Simbad)
Write:	<<[ASG2012] NNNN>>
N:	25
Object:	Poss. Cluster of * (SIMBAD class: Cluster*_Candidate = Cluster of Stars Candidate)
Note:	N=25 cluster candidates in a ring-like clster complex in NGC 2146. Use of data from the Snapshot Hubble U-band Cluster Survey (SHUCS).
in source:	NGC 2146
Ref:	=2012MNRAS.426.1185A
by	ADAMO A. , SMITH L.J., GALLAGHER J.S., BASTIAN N., RYON J., WESTMOQUETTE M.S., KONSTANTOPOULOS I.S., ZACKRISSON E., LARSEN S.S., SILVA-VILLA E., CHARLTON J.C., WEISZ D.R.
	Mon. Not. R. Astron. Soc., 426, 1185-1194 (2012)
	Revealing a ring-like cluster complex in a tidal tail of the starburst galaxy NGC 2146.
o	Table 1: <[ASG2012] NNNN> N=25 among (Nos 162-192, 3156-3159).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ASh
ASh	(Ambartsumian+Schachbazian) (Not yet in Simbad)
*****	Avoid the usage of ASh, prefer [AS58]
Details on Acronym: [ASK2006]
[ASK2006]	(Adelberger+Steidel+Kollmeier+, 2006)
Write:	<<[ASK2006] Q1549-ANN>> <<[ASK2006] QSO J1551+1910 abs N.NNNN>>
N:	1+1
Object:	QSO + DLA (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	A faint QSO that lies just 49" from the much brighter QSO HS 1549+1919 is identified. This QSO is designated as Q1549-D10 by the authors, also QSO J1551+1910 in SIMBAD. A DLA is found in the spectrum of this QSO.
Ref:	=2006ApJ...637...74A
by	ADELBERGER K.L. , STEIDEL C.C., KOLLMEIER J.A., REDDY N.A.
	Astrophys. J., 637, 74-79 (2006)
	Possible detection of Lyα fluorescence from a damped Lyα system at redshift z ~ 2.8.
o	<[ASK2006] Q1549-D10> N=1. <[ASK2006] QSO J1551+1910 abs 2.8420> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ASK2013]
[ASK2013]	(Assef+Stern+Kochanek+, 2013)
Write:	<<[ASK2013] JHHMMSS.ss+DDMMSS.s>>
N:	140
Object:	G (SIMBAD class: Galaxy)
Note:	Keck DEIMOS/LRIS spectroscopic observations of N=140 galaxies in the NOAO Deep Wide-Field Survey Bootes field.
Ref:	=2013ApJ...772...26A
by	ASSEF R.J. , STERN D., KOCHANEK C.S., BLAIN A.W., BRODWIN M., BROWN M.J.I., DONOSO E., EISENHARDT P.R.M., JANNUZI B.T., JARRETT T.H., STANFORD S.A., TSAI C.-W., WU J., YAN L.
	Astrophys. J., 772, 26 (2013)
	Mid-infrared selection of active galactic nuclei with the Wide-field Infrared Survey Explorer. II. Properties of WISE-selected active galactic nuclei in the NDWFS Bootes field.
o	Table 6: <[ASK2013] JHHMMSS.ss+DDMMSS.s> N=140.
=E=	Catalogue in electronic form as J/ApJ/772/26
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ASK2018]
[ASK2018]	(Anguita+Schechter+Kuropatkin+, 2018)
Write:	<<[ASK2018] DES JHHMM+DDMM>> <<[ASK2018] DES JHHMM+DDMM source N>> <<[ASK2018] DES JHHMM+DDMM A>>
N:	34+30+39
Object:	Poss. Grav. lens system + Poss. QSO + Poss. Grav. lensed image + Poss. Grav. lens (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=30 background sources and N=39 gravitationally lensed images in N=34 gravitational lens system candidates in the Dark Energy Survey. Follow-up observations with NTT EFOSC, Magellan IMACS, Keck ESI, and SOAR SAMI.
Ref:	=2018MNRAS.480.5017A
by	ANGUITA T. , SCHECHTER P.L., KUROPATKIN N., MORGAN N.D., OSTROVSKI F., ABRAMSON L.E., AGNELLO A., APOSTOLOVSKI Y., FASSNACHT C.D., HSUEH J.W., MOTTA V., ROJAS K., RUSU C.E., TREU T., WILLIAMS P., AUGER M., BUCKLEY-GEER E., LIN H., McMAHON R., ABBOTT T.M.C., ALLAM S., ANNIS J., BERNSTEIN R.A., BERTIN E., BROOKS D., BURKE D.L., CARNERO ROSELL A., CARRASCO-KIND M., CARRETERO J., CUNHA C.E., D'ANDREA C.B., DE VICENTE J., DEPOY D.L., DESAI S., DIEHL H.T., DOEL P., FLAUGHER B., GARCIA-BELLIDO J., GERDES D.W., GRUEN D., GRUENDL R.A., GSCHWEND J., HARTLEY W.G., HOLLOWOOD D.L., HONSCHEID K., JAMES D.J., KUEHN K., LIMA M., MAIA M.A.G., MIQUEL R., PLAZAS A.A., SANCHEZ E., SCARPINE V., SMITH M., SOARES-SANTOS M., SOBREIRA F., SUCHYTA E., TARLE G., WALKER A.R.
	Mon. Not. R. Astron. Soc., 480, 5017-5028 (2018)
	The STRong lensing Insights into the Dark Energy Survey (STRIDES) 2016 follow-up campaign - II. New quasar lenses from double component fitting.
o	Table 2: <[ASK2018] DES JHHMM+DDMM> N=34, <[ASK2018] DES JHHMM+DDMM source> N=22, <[ASK2018] DES JHHMM+DDMM source N> N=8. Figs 1-8, Tables 3-6: <[ASK2018] DES JHHMM+DDMM A> N=39.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ASKAP
ASKAP	(Australian Square Kilometer Array Pathfinder) (Not yet in Simbad)
*****	Avoid the usage of ASKAP, prefer [DSM2019]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ASKAP
ASKAP	(Australian Square Kilometer Array Pathfinder)
*****	Avoid the usage of ASKAP, prefer [WKM2021]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ASL2000]
[ASL2000]	(Altieri+Schartel+Lumb+, 2000)
Write:	<<[ASL2000] SN>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of GRB 001025 field: two sources are found in the IPN/RXTE error box.
Ref:	=2000GCN...884....1A
by	ALTIERI B. , SCHARTEL N., LUMB D., PIRO L., PARMAR A.
	GRB Coordinates Network, Circular Service, 884, 1-None (2000)
	CORRECTION to XMM-Newton observation of GRB 001025.
o	<[ASL2000] SN> (Nos S1-S2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ASM
ASM	(All Sky Monitor)
Write:	<<NAME ASM HHMM+DD>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Often found in the literature for Ginga 2000+25 = NAME ASM 2000+25
Ref:	=1988IAUC.4605....0S
by	SHRADER C.R.
	IAU Circ., -1-None (1988)
	ASM 2000+25.
o	<NAME ASM 2000+25>
Details on Acronym: [ASM2018]
[ASM2018]	(Agnello+Schechter+Morgan+, 2018)
Write:	<<[ASM2018] A JHHMM+DDMM>> <<[ASM2018] S JHHMM+DDMM>> <<[ASM2018] WGA JHHMM+DDMM>> <<[ASM2018] A J0140-1152 A>> <<[ASM2018] AHHMM+DDMM>> (not recognised by Simbad, but found in literature) <<[ASM2018] SHHMM+DDMM>> <<[ASM2018] WGAHHMM+DDMM>> <<[ASM2018] A0140-1152 A>>
N:	29+4+11+3
Object:	Poss. Grav. lens system + Poss. Pair of QSOs + Grav. lensed image of a QSO + Grav. lens (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	A quasar lens search in the ATLAS-DR3 public footprint. NOT ALFOSC, NTT EFOSC, and Magellan IMACS spectroscopy. Use of ATLAS-DR2, ATLAS-DR3, SDSS, WISE, and Gaia data.
Ref:	=2018MNRAS.475.2086A
by	AGNELLO A. , SCHECHTER P.L., MORGAN N.D., TREU T., GRILLO C., MALESANI D., ANGUITA T., APOSTOLOVSKI Y., RUSU C.E., MOTTA V., ROJAS K., CHEHADE B., SHANKS T.
	Mon. Not. R. Astron. Soc., 475, 2086-2096 (2018)
	Quasar lenses and pairs in the VST-ATLAS and Gaia.
o	Tables 1+4: <[ASM2018] A JHHMM+DDMM> N=24+5, <[ASM2018] S JHHMM+DDMM> N=4, <[ASM2018] WGA JHHMM+DDMM> N=11. Table 2: <[ASM2018] A J0140-1152 A> (Nos A-B, G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ASM98]
[ASM98]	(Armus+Soifer+Murphy+, 1998)
Write:	<<[ASM98] GN>> <<[ASM98] Star A>> <<[ASM98] Object NN>>
N:	8+3+4
Object:	G + * + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Objects in the field of the radio galaxy 4C +19.71: N=8 galaxies (Nos G1-G8), , N=3 stars (Nos Star A to Star C), N=4 other objects (Nos 9-12)
Ref:	=1998ApJ...495..276A
by	ARMUS L. , SOIFER B.T., MURPHY T.W., NEUGEBAUER G., EVANS A.S., MATTHEWS K.
	Astrophys. J., 495, 276-283 (1998)
	The [O III] emission-line nebula of the z = 3.594 radio galaxy 4C +19.71.
o	p. 277: components a and b = [ER96] MG 2141+192 a and b
o	Table 1: <[ASM98] GN> (Nos G1-G8), <[ASM98] Star A> (Nos A-C), <[ASM98] Object NN> (Nos 9-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Aso
Aso	(Aso+)
Note:	N=18 H13CO+ dense cores in OMC 2, OMC3 region.
*****	Avoid the usage of Aso, prefer [ATS2000]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ASP03
ASP03	(Alexov+Silva+Pierce, 2003)
Write:	<<ASP03 NNNN>>
N:	5992
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	KPNO observations. Wide-field UBVI images of the cluster ClG 0024+1654.
in source:	ClG 0024+1652 = HMS 0024+1654
Ref:	=2003AJ....126.2644A
by	ALEXOV A. , SILVA D.R., PIERCE M.J.
	Astron. J., 126, 2644-2661 (2003)
	A wide-field, broadband imaging survey of Butcher-Oemler cluster Cl 0024+1654: the catalog.
o	Catalog: <ASP03 NNNN> (Nos 1-5992).
=E=	Catalogue in electronic form as J/AJ/126/2644
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ASPECS
ASPECS	(ALMA SPECtroscopic Survey)
*****	Avoid the usage of ASPECS, prefer [ADW2016]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ASPECS
ASPECS	(ALMA SPECtroscopic Survey)
Write:	<<ASPECS LP.3mm.NN>> <<ASPECS LP.3mm.CNN>> <<ASPECS LP-MP.3mm.NN>> <<ASPECS LP.1mm.CNNa>> <<ASPECS LP.1mm.Faint.CNN>> <<ASPECS -LP.3mm.NN>> (not recognised by Simbad, but found in literature) <<ASPECS -LP-3mm.CNN>> <<ASPECS -LP-MP.3mm.NN>>
N:	16+6+2+36+26
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	ALMA band 3 (3mm) and band 6 (1.2mm) observations of N=16 CO-emitting galaxies (format LP.3mm.NN), N=6 continuum source candidates (format LP.3mm.CNN), and N=2 "MUSE prior" sources (format LP-MP.3mm.NN), and N=36+26 continuum sources candidates (formats LP.1mm.CNNa and LP.1mm.Faint.CNN), as part of the ALMA Spectroscopic Survey Large Program (ASPECS-LP), targeting the Hubble Ultra Deep Field (HUDF). See also [WDA2016] and [ADW2016] for the ASPECS pilot program.
Rem:	(a dash between the acronym and its contents is found in the literature)
in source:	NAME Hubble Ultra Deep Field
Ref:	=2019ApJ...882..136A
by	ARAVENA M. , DECARLI R., GONZALEZ-LOPEZ J., BOOGAARD L., WALTER F., CARILLI C., POPPING G., WEISS A., ASSEF R.J., BACON R., BAUER F.E., BERTOLDI F., BOUWENS R., CONTINI T., CORTES P.C., COX P., DA CUNHA E., DADDI E., DIAZ-SANTOS T., ELBAZ D., HODGE J., INAMI H., IVISON R., LE FEVRE O., MAGNELLI B., OESCH P., RIECHERS D., SMAIL I., SOMERVILLE R.S., SWINBANK A.M., UZGIL B., VAN DER WERF P., WAGG J., WISOTZKI L.
	Astrophys. J., 882, 136-136 (2019)
	The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: evolution of the molecular gas in CO-selected galaxies.
o	Fig. 14, Tables 1-3: <ASPECS LP.3mm.NN> (Nos 1-16).
Ref:	=2019ApJ...882..139G
by	GONZALEZ-LOPEZ J. , DECARLI R., PAVESI R., WALTER F., ARAVENA M., CARILLI C., BOOGAARD L., POPPING G., WEISS A., ASSEF R.J., BAUER F.E., BERTOLDI F., BOUWENS R., CONTINI T., CORTES P.C., COX P., DA CUNHA E., DADDI E., DIAZ-SANTOS T., INAMI H., HODGE J., IVISON R., LE FEVRE O., MAGNELLI B., OESCH P., RIECHERS D., RIX H.-W., SMAIL I., SWINBANK A.M., SOMERVILLE R.S., UZGIL B., VAN DER WERF P.
	Astrophys. J., 882, 139-139 (2019)
	The Atacama Large Millimeter/submillimeter Array SPECtroscopic Survey in the Hubble Ultra Deep Field: CO emission lines and 3 mm continuum sources.
o	Table 7: <ASPECS -LP.3mm.CNN> (Nos C01-C06).
Ref:	=2019ApJ...882..140B
by	BOOGAARD L.A. , DECARLI R., GONZALEZ-LOPEZ J., VAN DER WERF P., WALTER F., BOUWENS R., ARAVENA M., CARILLI C., BAUER F.E., BRINCHMANN J., CONTINI T., COX P., DA CUNHA E., DADDI E., DIAZ-SANTOS T., HODGE J., INAMI H., IVISON R., MASEDA M., MATTHEE J., OESCH P., POPPING G., RIECHERS D., SCHAYE J., SCHOUWS S., SMAIL I., WEISS A., WISOTZKI L., BACON R., CORTES P.C., RIX H.-W., SOMERVILLE R.S., SWINBANK M., WAGG J.
	Astrophys. J., 882, 140-140 (2019)
	The ALMA spectroscopic survey in the HUDF: nature and physical properties of gas-mass selected galaxies using MUSE spectroscopy.
o	Fig. 4, Table 2: <ASPECS LP-MP.3mm.NN> (Nos 01-02).
Ref:	=2020ApJ...897...91G
by	GONZALEZ-LOPEZ J. , NOVAK M., DECARLI R., WALTER F., ARAVENA M., CARILLI C., BOOGAARD L., POPPING G., WEISS A., ASSEF R.J., BAUER F.E., BOUWENS R., CORTES P.C., COX P., DADDI E., DA CUNHA E., DIAZ-SANTOS T., IVISON R., MAGNELLI B., RIECHERS D., SMAIL I., VAN DER WERF P., WAGG J.
	Astrophys. J., 897, 91-91 (2020)
	The ALMA Spectroscopic Survey in the HUDF: Deep 1.2 mm continuum number counts.
o	Fig. 2, Table 1: <ASPECS LP.1mm.CNNa> (Nos C01-C13, C14a-C14b, C15-C34). Table 5: <ASPECS LP.1mm.Faint.CNN> (Nos C01-C26).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ASPECS
ASPECS	(ALMA SPECtroscopic Survey)
*****	Avoid the usage of ASPECS, prefer [WDA2016]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ASR
ASR	(Aspin+Sandell+Russell)
Write:	<<ASR NNN>>
N:	134
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	NGC 1333
Ref:	=1994A&AS..106..165A
by	ASPIN C. , SANDELL G., RUSSELL A.P.G.
	Astron. Astrophys., Suppl. Ser., 106, 165-198 (1994)
	Near-IR imaging photometry of NGC 1333. I. The embedded PMS stellar population.
o	SSV = [SVS76] NGC 1333, HJ = [HJ83], S86 = SSWMW, IRAS = [JCC87]
o	<ASR NNN> (Nos 1-134). <Em* LkHA NNNa> (No. 352A).
=E=	Catalogue in electronic form as <J/A+AS/106/165/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ASR2016]
[ASR2016]	(Alavi+Siana+Richard+, 2016)
Write:	<<[ASR2016] a.N>>
N:	15
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC3 observations of N=15 lensed images in the field of the galaxy cluster ACO 1689.
in source:	ACO 1689
Ref:	=2016ApJ...832...56A
by	ALAVI A. , SIANA B., RICHARD J., RAFELSKI M., JAUZAC M., LIMOUSIN M., FREEMAN W.R., SCARLATA C., ROBERTSON B., STARK D.P., TEPLITZ H.I., DESAI V.
	Astrophys. J., 832, 56-56 (2016)
	The evolution of the faint end of the UV luminosity function during the peak epoch of star formation (1 < z < 3).
o	Table 5: <[ASR2016] a.N> N=15 among (Nos a.1-a.4 to e.1-e.4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ass
Ass	(Stellar Association)= Assoc
Write:	<<Ass CCC A N>> <<Ass CCC A N.NN>> <<Ass CCC OB N>> <<Ass CCC OB Na>> <<Ass CCC OB NaN>> <<Ass CCC OB N.NN>> <<Ass CCC OB NAA>> <<Ass CCC OB NWW>>
Object:	Assoc. (SIMBAD class: Association = Association of Stars)
Note:	In SIMBAD only. To find the designation as in the literature, drop the first word (Ass). Format ending as 'Na' and 'NaN' is found the first time in 1977ApJS...34..115W . Format ending as 'N.N' is found the first time in 1993A&AS..100..501T, using the distance as a parameter in the the numbering '.N' Format ending as 'N.NN' is found the first time in 1996AJ....111..306T
Ref:	=1977ApJS...34..115W
by	WARREN W.H. , HESSER J.E.
	Astrophys. J., Suppl. Ser., 34, 115-206 (1977)
	A photometric study of the Ori OB1 association. I. Observational data.
o	Table 1: <WH NNN> (Nos 1-526). Table 10: <Ass Ori OB 1a> (Nos 1a-1e), <Ass Ori OB 1aN> (Nos 1b1-1b3, 1c1-1c4, 1d1).
Ref:	=1993A&AS..100..501T
by	TOVMASSIAN H.M. , HOVHANNESSIAN R.K., EPREMIAN R.A., HUGUENIN D.
	Astron. Astrophys., Suppl. Ser., 100, 501-515 (1993)
	Bright blue stars in Vela observed with the "Glazar" space telescope.
o	Table 1, 1ere col.: <Glazar Vel NN> (Nos 1-71), 2eme col.: <Glazar HHMM+DD.N> N=2. Text: <Ass CCC A N.N>, <Ass CCC OB N.N> 1st ref. with this format.
Ref:	=1995PAZh...21...13M
by	MEL'NIK A.M. , EFREMOV Y.N.
	Pis'ma Astron. Zh., 21, 13-30 (1995)
	New list of OB associations of our galaxy.
o	Table 1: <Ass CCC OB NA> N=37, <Ass Ara OB 1AA> (Nos AA, AB). Table 1: <[ME95] Cyg 1-8-9> N=1, <[ME95] Car 1-2> N=1, <[ME95] CLUST N> (Nos 1-5).
Ref:	=1996AJ....111..306T
by	TOVMASSIAN H.M. , NAVARRO S.G., CARDONA O.
	Astron. J., 111, 306-314 (1996)
	OB stellar association in Crux. II. Analysis and discussion.
o	<Ass Cru B N.NN> N=8
=E=	Catalogue in electronic form as <J/PAZh/21/13/>
=E=	Catalogue in electronic form as <II/36/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ass
Ass	(Stellar Association)= Assoc
Write:	<<Ass CCC OB N-NN>>
Object:	* in Assoc. (SIMBAD class: Star)
Note:	In SIMBAD only.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ass Cha T
Ass Cha T	(Assoc Chamaeleon T)= (Cha) = (HM) = (HMEN)
Write:	<<Ass Cha T 1-NN>>
N:	32
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Note:	List 1 in Association Cha T.
in source:	NAME Cha T Association
Ref:	=1973ApJ...180..115H
by	HENIZE K.G. , MENDOZA E.E.
	Astrophys. J., 180, 115-119 (1973)
	Emission-line stars in the Chamaeleon T association.
o	<Ass CHA T 1-NN> (Nos 1-32)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ass Cha T
Ass Cha T	(Assoc Chamaeleon T)= (Cha) = (T) = (WKK)
Write:	<<Ass Cha T 2-NN>>
N:	56
Object:	* in Assoc. (SIMBAD class: Star)
Note:	Table 5: often found with format 'TNN', with prefixe T for members of the T asociation. Format '2-NN': List 2 in Association Cha T. See also: WKK, [PCW91], [AWW90].
in source:	NAME Cha T Association
Ref:	=1987MNRAS.224..497W
by	WHITTET D.C.B. , KIRRANE T.M., KILKENNY D., OATES A.P., WATSON F.G., KING D.J.
	Mon. Not. R. Astron. Soc., 224, 497-512 (1987)
	A study of the Chamaeleon dark cloud and T-association -I.Extinction, distance and membership.
o	Table 5: <ASS CHA T 2-NN> N=56, Table 6: <WKK FNN> N=54
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ass Cyg OB 2-
Ass Cyg OB 2-	(Assoc. Cyg OB 2)
*****	Avoid the usage of Ass Cyg OB 2-, prefer [MM53]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ass Cyg OB 2-
Ass Cyg OB 2-	(Assoc. Cyg OB 2)
*****	Avoid the usage of Ass Cyg OB 2-, prefer RLP
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ass Cyg OB 2-
Ass Cyg OB 2-	(Assoc. Cyg OB 2)
*****	Avoid the usage of Ass Cyg OB 2-, prefer Schulte
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [ASS79]
[ASS79]	(Adams+Strom+Strom, 1979)= (HH)
Write:	<<[ASS79] NGC 2264 HH NN-N>>
N:	5
Object:	HH (SIMBAD class: HerbigHaroObj = Herbig-Haro Object)
Note:	HH objects associated with NGC 2264. The authors use a format 'NGC 2264 NN-N' for these objects Identif. charts in Fig.2
in source:	NGC 2264
Ref:	=1979ApJ...230L.183A
by	ADAMS M.T. , STROM K.M., STROM S.E.
	Astrophys. J., 230, 183-186 (1979)
	Herbig-Haro objects associated with NGC 2264.
o	Table 1: <[ASS79] NGC 2264 HH NN-N> N=5
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ASS80]
[ASS80]	(Adams+Strom+Strom, 1980)
Write:	<<[ASS80] ACO NNNN NN>>
N:	357
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Table 3: N=58 G in ACO 76, format 'ACO 76 NN' Table 4: N=45 G in ACO 179, format 'ACO 179 NN' Table 5: N=43 G in ACO 194, format 'ACO 194 NN' Table 6: N=44 G in ACO 195, format 'ACO 195 NN' Table 7: N=44 G in ACO 999, format 'ACO 999 NN' Table 8: N=50 G in ACO 1016, format 'ACO 1016 NN'
in source:	ACO 76
in source:	ACO 179
in source:	ACO 194
in source:	ACO 195
in source:	ACO 999
in source:	ACO 1016
Ref:	=1980ApJ...238..445A
by	ADAMS M.T. , STROM K.M., STROM S.E.
	Astrophys. J., 238, 445-457 (1980)
	Linear clusters of galaxies.
o	Table 3: <[ASS80] ACO 76 NN> N=58, Table 4: <[ASS80] ACO 179 NN> N=45, Table 5: <[ASS80] ACO 194 NN> N=43, Table 6: <[ASS80] ACO 195 NN> N=44, Table 7: <[ASS80] ACO 999 NN> N=44, Table 8: <[ASS80] ACO 1016 NN> N=50
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ASS83]
[ASS83]	(Adams+Strom+Strom, 1983)= (VC) (Not yet in Simbad)
Write:	<<[ASS83] NN-NN>>
N:	160
Object:	Em. Obj. (SIMBAD class: EmLine* = Emission-line Star)
Note:	N=160 emission objects in the field of NGC 2264. In the format 'NN-NN' the first 2 digits stands for frame (Nos 1-30), the last 2 digits for oject number in each frame.
in source:	NGC 2264
Ref:	=1983ApJS...53..893A
by	ADAMS M.T. , STROM K.M., STROM S.E.
	Astrophys. J., Suppl. Ser., 53, 893-935 (1983)
	The star-forming history of the young cluster NGC 2264.
o	Table 6: <Cl* NGC 2419 ASS N> (Nos 1-3, 5). Tables 6, 7, 13-18: <Cl* NGC 2264 ASS NNN> N=47+240. Table 11: <[ASS83] NN-NN> N=160.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ASS84]
[ASS84]	(Arp+Surdej+Swings, 1984)
Write:	<<[ASS84] NGC 470 NNA>>
N:	3
Object:	QSO (SIMBAD class: QSO = Quasar)
Note:	QSOs near NGC 470.
Ref:	=1984A&A...138..179A
by	ARP H. , SURDEJ J., SWINGS J.P.
	Astron. Astrophys., 138, 179-182 (1984)
	Two quasars seen near the spiral galaxy NGC 470.
o	<[ASS84] NGC 470 NNA> (Nos 68, 68D, 76)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ASS97]
[ASS97]	(Alksnis+Sharov+Shokin+, 1997)
Write:	<<[ASS97] N>>
N:	6
Object:	Comparison * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1997IBVS.4491....1A
by	ALKSNIS A. , SHAROV A.S., SHOKIN Y.A., EVSTIGNEEVA N.M.
	IAU Inform. Bull. Var. Stars, 4491, 1-2 (1997)
	More flares of HY Andromedae.
o	Table 2: <[ASS97] N> (Nos 1-6)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Assoc
Assoc	(Association) (Not yet in Simbad)
Write:	<<Assoc NN>> <<Assoc NN.N>>
N:	89
Object:	Assoc. (SIMBAD class: Association = Association of Stars)
Ref:	=1970CSCA..C......0A
by	ALTER G. , RUPRECHT J., VANYSEK V.
	Catalogue of star clusters and associations + supplements. Akad. Kiado, Budapest, Hungary, 3086 p., 2nd edition,1970, 0-None (1970)
	Catalogue of star clusters and associations + supplements.
o	<Assoc NN.N>. <GCl NNN.N>. <OCl NNNN.N>.
Ref:	=1981CSCAS.C......0R
by	RUPRECHT J. , BALAZS B., WHITE R.E.
	Akad. Kiado, Budapest, Hungary,1981, 0-None (1981)
	Catalogue of star clusters and associations. Suppl. 1 to the 2nd edition.
o	<Assoc NN.N> (Nos 1-70), N=89. <GCl NNN.N> (Nos 1-125), N=137. <OCl NNNN.N> (Nos 1-1044) N=1112.
=E=	Catalogue in electronic form as VII/31
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Assoc
Assoc	(Stellar Associations)
====>	Equivalent to: Ass
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AST2006]
[AST2006]	(Ajiki+Shioya+Taniguchi+, 2006)
Write:	<<[AST2006] NN>>
Object:	LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Search for Emission-line galaxies at low redshifts around SDSS J104433.04-012502.2 with Subaru Suprime-Cam.
Ref:	=2006PASJ...58..113A
by	AJIKI M. , SHIOYA Y., TANIGUCHI Y., MURAYAMA T., NAGAO T., SASAKI S.S., SUMIYA R., MORIOKA T., HATAKEYAMA Y., YOKOUCHI A., TAKAHASHI M.I., KOIZUMI O.
	Publ. Astron. Soc. Jap., 58, 113-130 (2006)
	Strong emission-line galaxies at low redshifts in the field around the quasar SDSSp J104433.04-012502.2.
o	Tables 1, 2: <[AST2006] NN> (Nos 1-55).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AST3II
AST3II	(Second AST3 telescope) (Not yet in Simbad)
*****	Avoid the usage of AST3II, prefer [ZYL2019]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ASTEP
ASTEP	(Antarctica Search for Transiting ExoPlanets)
Write:	<<ASTEP A-NNN-NNNN-NNNN>> <<ASTEP V-NNNN>> <<ASTEP C-NN>>
N:	1829+43
Object:	V* + Poss. Planet (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	ASTEP 400 (a 40-cm telescope) is the main instrument of the ASTEP (Antarctica Search for Transiting ExoPlanets) programme. N=1829 variable stars and N=43 planetary transit candidates. For more information, visit https://astep-vo.oca.eu/
Ref:	=2016ApJS..226...21C
by	CHAPELLIER E. , MEKARNIA D., ABE L., GUILLOT T., AGABI K., RIVET J.-P., SCHMIDER F.-X., CROUZET N., ARISTIDI E.
	Astrophys. J., Suppl. Ser., 226, 21-21 (2016)
	A catalog of eclipsing binaries and variable stars observed with ASTEP 400 from Dome C, Antarctica.
o	Tables 2-3, col(1): <ASTEP V-NNNN> (Nos V-1 to V-1829) = Tables 2-3, col(2): <ASTEP A-NNN-NNNN-NNNN> N=673+1156.
Ref:	=2016MNRAS.463...45M
by	MEKARNIA D. , GUILLOT T., RIVET J.-P., SCHMIDER F.-X., ABE L., GONCALVES I., AGABI A., CROUZET N., FRUTH T., BARBIERI M., BAYLISS D.D.R., ZHOU G., ARISTIDI E., SZULAGYI J., DABAN J.-B., FANTEI-CAUJOLLE Y., GOUVRET C., ERIKSON A., RAUER H., BOUCHY F., GERAKIS J., BOUCHEZ G.
	Mon. Not. R. Astron. Soc., 463, 45-62 (2016)
	Transiting planet candidates with ASTEP 400 at Dome C, Antarctica.
o	Tables 4-5, col(1): <ASTEP C-NN> (Nos C-1 to C-43) = Tables 4-5, col(2): <ASTEP A-NNN-NNNN-NNNN> N=43.
=E=	Catalogue in electronic form as <J/ApJS/226/21/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ASU2006]
[ASU2006]	(Adami+Scheidegger+Ulmer+, 2006)
Write:	<<[ASU2006] NNN>>
N:	735
Object:	G (SIMBAD class: Galaxy)
Note:	CFHT CFH12K camera observations of the Coma cluster field.
in source:	Coma Cluster = ACO 1656
Ref:	=2006A&A...459..679A
by	ADAMI C. , SCHEIDEGGER R., ULMER M., DURRET F., MAZURE A., WEST M.J., CONSELICE C.J., GREGG M., KASUN S., PELLO R., PICAT J.P.
	Astron. Astrophys., 459, 679-692 (2006)
	A deep wide survey of faint low surface brightness galaxies in the direction of the Coma cluster of galaxies.
o	Table 1: <[ASU2006] NNN> (Nos 1-735).
=E=	Catalogue in electronic form as J/A+A/459/679
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ASV
ASV	(Atlas Stellarum Variabilium) (Not yet in Simbad)
Write:	<<ASV FFFF-NNN>> <<ASV V NNNN CCC>>
Object:	* (SIMBAD class: Star)
Note:	Use standard-names. Type of object: sequences of stars around variables stars.
Ref:	=1899ASV...C......0H
by	HAGEN I.G.
	BEROLINI (Roma ?, Washington) Ed., First serie (several series, several years, several authors), 0-None (1899)
	Atlas Stellarum Variabilium.
o	<ASV FFFF-NNN>
Details on Acronym: ASV
ASV	(Angonin-Willaime+Soucail+Vanderriest)
Write:	<<ASV NN>>
N:	38
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Ref:	=1994A&A...291..411A
by	ANGONIN-WILLAIME M.-C. , SOUCAIL G., VANDERRIEST C.
	Astron. Astrophys., 291, 411-419 (1994)
	Gravitational lensing of Q 0957+561: a study of the cluster at z=0.355.
o	p. 412, S95132=SA 95-132 , G16350=G 163-50
o	Table 2: <ASV NN> (Nos 1-38)
Origin	of the Acronym: L (Veron)
Details on Acronym: [ASV69]
[ASV69]	(Andrievski+Spangenberg+Valtz+, 1969)= (Cri) (Not yet in Simbad)
Write:	<<[ASV69] NNN>>
N:	130
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1969ATsir.494....1A
by	ANDRIEVSKI A.E. , SPANGENBERG E.E., VALTZ I.E., GINDILIS L.M., GORSHKOV A.G., IVANOV V.N., KONNIKOVA V.K., KURILCHIK V.N., LARIONOV M.G., MOISEEV I.G., NIKITIN V.V., PORTMAN V.I., SOGLASNOV V.A.
	Astron. Tsirk., 494, 1-3 (1969)
	Flux densities of discrete radio sources at 3.5 cm wavelength.
o	Table 1: <[ASV69] NNN> (Nos 1-130)
Details on Acronym: ASW
ASW	(Ardeberg+Sarg+Wramdemark)
Write:	<<ASW R-NN>>
N:	121
Object:	* (SIMBAD class: Star)
Note:	In the format 'R', roman numeral, stands for objects in Tables I to IV. Finding charts
Ref:	=1973A&AS....9..163A
by	ARDEBERG A. , SARG K., WRAMDEMARK S.
	Astron. Astrophys., Suppl. Ser., 9, 163-181 (1973)
	Photoelectric UBV photometry in four areas of intermediate-high galactic latitude.
o	<ASW F-NN> N=121
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [ASW79]
[ASW79]	(Arp+Sargent+Willis+, 1979)
Write:	<<[ASW79] N>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Note:	N=3 galaxies North of 6W 0846+51W1.
Ref:	=1979ApJ...230...68A
by	ARP H. , SARGENT W.L.W., WILLIS A.G., OOSTERBAAN C.E.
	Astrophys. J., 230, 68-78 (1979)
	An eruptive BL Lacertae object with a high redshift, 0846+51W1.
o	Fig.1, Table 1: <[ASW79] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ASW90]
[ASW90]	(Akujor+Spencer+Wilkinson, 1990)
Write:	<<[ASW90] 3C 147 Aa>> <<[ASW90] 3C 295 Aa>>
N:	6+3
Object:	Radio component (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio structures of 3C 147 and 3C 295. In the format, the letter 'e' stands for 'extension'. For 3C 147 see also [RW80].
in source:	3C 147
in source:	3C 295
Ref:	=1990MNRAS.244..362A
by	AKUJOR C.E. , SPENCER R.E., WILKINSON P.N.
	Mon. Not. R. Astron. Soc., 244, 362-366 (1990)
	MERLIN images of two compact steep-spectrum sources, 3C 147 and 295.
o	Fig.1: <[ASW90] 3C 147 Aa> (Nos A-D, Ae, Be). Fig.2: <[ASW90] 3C 295 Aa> (Nos A-B, Be).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ASW98]
[ASW98]	(AbdelSalam+Saha+Williams, 1998) (Not yet in Simbad)
Write:	<<[ASW98] a>> <<[ASW98] aN>>
N:	4+11
Object:	Arclet (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=4 'arc system' (Nos a-d), each with merging images or 'arclet' (Nos a1-a2, b1-b3, c1-c3, d1-d3). See also LPS
in source:	ACO 2218
Ref:	=1998AJ....116.1541A
by	ABDELSALAM H.M. , SAHA P., WILLIAMS L.L.R.
	Astron. J., 116, 1541-1552 (1998)
	Nonparametric reconstruction of Abell 2218 from combined weak and strong lensing.
o	<[ASW98] a> (Nos a-d), <[ASW98] aN> (Nos a1-a2, b1-b3, c1-c3, d1-d3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ASXDF
ASXDF	(ALMA Subaru XMM-Newton Deep Field)
Write:	<<ASXDF NNNN.NNN.NA>>
N:	13+70
Object:	smm G (SIMBAD class: Galaxy)
Note:	ALMA 1.1mm continuum observations of N=13+70 submillimeter galaxies (SMGs) at z~>3. Use of AzTEC data.
Ref:	=2015ApJ...810..133I
by	IKARASHI S. , IVISON R.J., CAPUTI K.I., ARETXAGA I., DUNLOP J.S., HATSUKADE B., HUGHES D.H., IONO D., IZUMI T., KAWABE R., KOHNO K., LAGOS C.D.P., MOTOHARA K., NAKANISHI K., OHTA K., TAMURA Y., UMEHATA H., WILSON G.W., YABE K., YUN M.S.
	Astrophys. J., 810, 133 (2015)
	Compact starbursts in z ~ 3-6 submillimeter galaxies revealed by ALMA.
o	Table 1: <ASXDF 1100.NNN.N> N=13 among (Nos 013.1-231.1).
Ref:	=2017ApJ...849L..36I
by	IKARASHI S. , CAPUTI K.I., OHTA K., IVISON R.J., LAGOS C.D.P., BISIGELLO L., HATSUKADE B., ARETXAGA I., DUNLOP J.S., HUGHES D.H., IONO D., IZUMI T., KASHIKAWA N., KOYAMA Y., KAWABE R., KOHNO K., MOTOHARA K., NAKANISHI K., TAMURA Y., UMEHATA H., WILSON G.W., YABE K., YUN M.S.
	Astrophys. J., 849L, 36-36 (2017)
	Very compact millimeter sizes for composite star-forming/AGN submillimeter galaxies.
o	Table 1: <ASXDF 1100.NNN.NA> N=69 among (Nos 002.1-252.1).
=E=	Catalogue in electronic form as <J/ApJ/849/L36/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AT
AT	(Astronomical Transient)
Write:	<<AT YYYYA>> <<AT YYYYaa>> <<AT YYYYaaa>> <<AT YYYYaaaa>>
Object:	Transient (SIMBAD class: Transient = Transient Event)
Note:	As of January 1, 2016, the Transient Name Server (TNS) is the official IAU mechanism for reporting new astronomical transients (ATs) such as supernova candidates. Once spectroscopically confirmed, new supernova discoveries are officially designated a SN name (of the form SN 2016A and so on, as before). This is a continuation of the IAU naming scheme for supernovae which was handled by the Central Bureau for Astronomical Telegrams until the end of 2015, and has been approved as the official IAU naming scheme by the IAU Executive Committee from 1st January 2016. For more information visit the Transient Name Server (TNS) at https://wis-tns.weizmann.ac.il/ See also SN.
Details on Acronym: AT
AT	(Ariel Transient)
Write:	<<AT HHMM+DDd>>
N:	27
Object:	(X) (SIMBAD class: X = X-ray Source)
Ref:	=1983MNRAS.205..875P
by	PYE J.P. , McHARDY I.M.
	Mon. Not. R. Astron. Soc., 205, 875-888 (1983)
	The Ariel V sky survey of fast-transient X-ray sources.
o	<AT HHMM+DDd> N=27
Details on Acronym: AT
AT	(ATCA)
*****	Avoid the usage of AT, prefer [SRE2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AT2000]
[AT2000]	(Aparicio+Tikhonov, 2000)= ([AT2000a]) (Not yet in Simbad)
Write:	<<[AT2000] N>>
N:	8
Object:	HII (SIMBAD class: HIIReg = HII Region)
in source:	DDO 190
Ref:	=2000AJ....119.2183A
by	APARICIO A. , TIKHONOV N.
	Astron. J., 119, 2183-2193 (2000)
	The spatial and age distribution of stellar populations in DDO 190.
o	Table 2, Fig.5: <[AT2000] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AT2000a]
[AT2000a]	(Aparicio+Tikhonov, 2000) (Not yet in Simbad)
*****	Avoid the usage of [AT2000a], prefer [AT2000]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AT2000b]
[AT2000b]	(Anthony-Twarog+Twarog, 2000)= (T)
Write:	<<[AT2000b] NNNN>>
N:	5137
Object:	* (SIMBAD class: Star)
Note:	CTIO 0.9m telescope photometric observations of NGC 6397.
in source:	NGC 6397
Ref:	=2000AJ....120.3111A
by	ANTHONY-TWAROG B.J. , TWAROG B.A.
	Astron. J., 120, 3111-3126 (2000)
	CCD uvbyHβ photometry in clusters. II. The nearest globular cluster, NGC 6397.
o	Table 2: <[AT2000b] NNNN> (Nos 1-5137).
=E=	Catalogue in electronic form as J/AJ/120/3111
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AT20G
AT20G	(Australia Telescope 20 GHz)
Write:	<<AT20G JHHMMSS.s+DDMMSS>> <<AT20G JHHMMSS+DDMMSS>>
N:	about 6000
Object:	(Rad) (SIMBAD class: cmRad = Centimetric Radio Source)
Note:	The Australia Telescope 20 GHz (AT20G) Survey is a blind survey of the whole Southern sky at 20 GHz (with follow-up observations at 5 and 8 GHz) carried out with the Australia Telescope Compact Array (ATCA) from 2004 to 2007. To date, it has completed the scan of the full Southern sky, detecting, down to a 50 mJy flux limit, more than 4400 sources below declination -15deg and expecting 1500 in the declination range -15deg dec <0deg for which the analysis is still on-going. Authors have performed near simultaneous observations of total intensity and polarization of the sources at 20, 8 and 5 GHz. 2008MNRAS.384..775M is the first ref. with AT20G objects. 2010MNRAS.402.2403M is the full source catalogue (version 1.0).
Ref:	=2008MNRAS.384..775M
by	MASSARDI M. , EKERS R.D., MURPHY T., RICCI R., SADLER E.M., BURKE S., DE ZOTTI G., EDWARDS P.G., HANCOCK P.J., JACKSON C.A., KESTEVEN M.J., MAHONY E., PHILLIPS C.J., STAVELEY-SMITH L., SUBRAHMANYAN R., WALKER M.A., WILSON W.E.
	Mon. Not. R. Astron. Soc., 384, 775-802 (2008)
	The Australia Telescope 20-GHz (AT20G) Survey: the Bright Source Sample.
o	Tables 2, 3, col(1): <[MEM2008] NNN> (Nos 1-320) = Tables 2, 3, col(2, 3): <AT20G JHHMMSS.s+DDMMSS> N=320.
Ref:	=2010MNRAS.402.2403M
by	MURPHY T. , SADLER E.M., EKERS R.D., MASSARDI M., HANCOCK P.J., MAHONY E., RICCI R., BURKE-SPOLAOR S., CALABRETTA M., CHHETRI R., DE ZOTTI G., EDWARDS P.G., EKERS J.A., JACKSON C.A., KESTEVEN M.J., LINDLEY E., NEWTON-McGEE K., PHILLIPS C., ROBERTS P., SAULT R.J., STAVELEY-SMITH L., SUBRAHMANYAN R., WALKER M.A., WILSON W.E.
	Mon. Not. R. Astron. Soc., 402, 2403-2423 (2010)
	The Australia Telescope 20 GHz Survey: the source catalogue.
o	at20gcat: <AT20G JHHMMSS+DDMMSS> N=5890.
=E=	Catalogue in electronic form as J/MNRAS/384/775
=E=	Catalogue in electronic form as J/MNRAS/402/2403
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [AT96]
[AT96]	(Artyukh+Tyul'bashev, 1996)
Write:	<<[AT96] HHMMSS+DDMM>> <<[AT96] HHMMSS+DDMM.m>>
N:	125
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	See also [ATI98]
Ref:	=1996ARep...40..601A
by	ARTYUKH V.S. , TYUL'BASHEV S.A.
	Astron. Rep., 40, 601-607 (1996)
	The cosmological evolution of compact radio sources from 102 MHz observations.
o	1996AZh....73..661A
o	Table 1: <[AT96] HHMMSS+DDMM>, <[AT96] HHMMSS+DDMM.m>, N=125
=E=	Catalogue in electronic form as VIII/67
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ATA2011]
[ATA2011]	(Annibali+Tosi+Aloisi+, 2011)
Write:	<<[ATA2011] NN>>
N:	81
Object:	Poss. Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations of N=81 star cluster candidates in NGC 4449.
in source:	NGC 4449
Ref:	=2011AJ....142..129A
by	ANNIBALI F. , TOSI M., ALOISI A., VAN DER MAREL R.P.
	Astron. J., 142, 129 (2011)
	The cluster population of the irregular galaxy NGC 4449 as seen by the Hubble Advanced Camera for Surveys.
o	The central super star cluster (SSC) (e.g. the first line of Table 1) is [GHG2001] 1 in SIMBAD.
o	Table 1: <[ATA2011] NN> (Nos 1-81).
=E=	Catalogue in electronic form as <J/AJ/142/129/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ATATS
ATATS	(Allen Telescope Array Twenty-cm Survey)
Write:	<<ATATS JHHMMSS+DDMMSS>>
N:	about 4408
Object:	Radio(cm) (SIMBAD class: Radio = Radio Source)
Note:	In preparation. A survey at 1.4 GHz with the Allen Telescope Array. A paper on the deep image of 690 square degrees of sky has been submitted, and a paper on the catalogs from the twelve individual epochs of data is in preparation. Preliminary results were presented at a recent meeting in Tucson - a link to the PDF of this presentation is below should this be useful: http://www.noao.edu/meetings/eventful-universe/Friday0319/croft_e_ventful.pdf
Ref:	=2010ApJ...719...45C
by	CROFT S. , BOWER G.C., ACKERMANN R., ATKINSON S., BACKER D., BACKUS P., BAROTT W.C., BAUERMEISTER A., BLITZ L., BOCK D., BRADFORD T., CHENG C., CORK C., DAVIS M., DE BOER D., DEXTER M., DREHER J., ENGARGIOLA G., FIELDS E., FLEMING M., FORSTER J.R., GUTIERREZ-KRAYBILL C., HARP G., HELFER T., HULL C., JORDAN J., JORGENSEN S., KEATING G., KILSDONK T., LAW C., VAN LEEUWEN J., LUGTEN J., MacMAHON D., McMAHON P., MILGROME O., PIERSON T., RANDALL K., ROSS J., SHOSTAK S., SIEMION A., SMOLEK K., TARTER J., THORNTON D., URRY L., VITOUCHKINE A., WADEFALK N., WELCH J., WERTHIMER D., WHYSONG D., WILLIAMS P.K.G., WRIGHT M.
	Astrophys. J., 719, 45-58 (2010)
	The Allen Telescope Array Twenty-centimeter Survey–A 690 °^{2}, 12 epoch radio data set. I. Catalog and long-duration transient statistics.
o	(Erratum) erratum vol.724, p.827 (2010)
o	Table 2: <ATATS JHHMMSS+DDMMSS> N=4408. UC Berkeley
=E=	Catalogue in electronic form as <VIII/87/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [ATB2004]
[ATB2004]	(Alonso-Herrero+Takagi+Baker+, 2004)
Write:	<<[ATB2004] CNN>> <<[ATB2004] CN'>>
N:	12+1
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST NICMOS observations of the central region of NGC 5253. N=12 stellar clusters, clusters C3 and C3' are heavily blended and form a double nuclear cluster.
in source:	NGC 5253
Ref:	=2004ApJ...612..222A
by	ALONSO-HERRERO A. , TAKAGI T., BAKER A.J., RIEKE G.H., RIEKE M.J., IMANISHI M., SCOVILLE N.Z.
	Astrophys. J., 612, 222-237 (2004)
	Obscured star formation in the central region of the dwarf galaxy NGC 5253.
o	Fig.2, Table 1: <[ATB2004] CNN> (Nos C1-C12), <[ATB2004] CN'> (No. C3').
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ATB2006]
[ATB2006]	(Aracil+Tripp+Bowen+, 2006)
Write:	<<[ATB2006] WWNN>> <<[ATB2006] WWNa>>
N:	32
Object:	G (SIMBAD class: Galaxy)
Note:	KPNO 4m telescope MOSA photometry and spectroscopy of galaxies in the field of QSO HS 0624+6907.
Ref:	=2006MNRAS.367..139A
by	ARACIL B. , TRIPP T.M., BOWEN D.V., PROCHASKA J.X., CHEN H.-W., FRYE B.L.
	Mon. Not. R. Astron. Soc., 367, 139-155 (2006)
	High-metallicity, photoionized gas in intergalactic large-scale filaments.
o	(Erratum) erratum vol. 372, p. 959 (2006)
o	Figs 1, 2, Table 2: <[ATB2006] WWNNa> (Nos SW1-SW3, SE1-SE13, NE1-NE3, NW1-NW3, NW4a-NW4b, NW5-NW12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ATCA
ATCA	(Australia Telescope Compact Array) (Not yet in Simbad)
*****	Avoid the usage of ATCA, prefer [WJK2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ATCA
ATCA	(Australia Telescope Compact Array)
*****	Avoid the usage of ATCA, prefer [FBR2002]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ATCA
ATCA	(Australia Telescope Compact Array)
*****	Avoid the usage of ATCA, prefer [GGM98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ATCA
ATCA	(Australia Telescope Compact Array)
*****	Avoid the usage of ATCA, prefer [GSF98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ATCA
ATCA	(Australia Telescope Compact Array)
*****	Avoid the usage of ATCA, prefer [KGJ2003]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ATCA-ADFS
ATCA-ADFS	(Australia Telescope Compact Array - AKARI Deep Field South)
Write:	<<ATCA-ADFS JHHMMSS+DDMMSS>>
N:	530
Object:	(Radio) (SIMBAD class: Radio = Radio Source)
Note:	ATCA 20cm observations of N=530 radio sources in a region containing the AKARI Deep Field South (ADF-S) near the South Ecliptic Pole (SEP).
Ref:	=2012MNRAS.427.1830W
by	WHITE G.J. , HATSUKADE B., PEARSON C., TAKAGI T., SEDGWICK C., MATSUURA S., MATSUHARA H., SERJEANT S., NAKAGAWA T., LEE H.M., OYABU S., JEONG W.-S., SHIRAHATA M., KOHNO K., YAMAMURA I., HANAMI H., GOTO T., MAKIUTI S., CLEMENTS D.L., MALEK K., KHAN S.A.
	Mon. Not. R. Astron. Soc., 427, 1830-1846 (2012)
	A deep ATCA 20 cm radio survey of the AKARI Deep Field South near the South Ecliptic Pole.
o	Table 2: <ATCA-ADFS JHHMMSS+DDMMSS> N=530.
=E=	Catalogue in electronic form as J/MNRAS/427/1830
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ATCDFS
ATCDFS	(Australia Telescope, CDFS field)
Write:	<<ATCDFS JHHMMSS.s+DDMMSSA>> <<ATCDFS JHHMMSS.ss+DDMMSS.s>>
N:	1600
Object:	G (SIMBAD class: Galaxy)
Note:	The Australia Telescope Large Area Survey (ATLAS) is a project to survey 6 sq deg in the southern sky with the Australia Telescope Compact Array (ATCA). In the ELAIS S1 field, see ATELAIS. See also [AMK2006], [NAA2006].
in source:	NAME CDFS
Ref:	=2006AJ....131.1216A
by	AFONSO J. , MOBASHER B., KOEKEMOER A., NORRIS R.P., CRAM L.
	Astron. J., 131, 1216-1230 (2006)
	Optical and X-ray identification of faint radio sources in the GOODS CDF-S Advanced Camera for Surveys field.
o	Table 1: <[AMK2006] NNa> N=72 (Nos 1-64) = <ATCDFS JHHMMSS.ss+DDMMSS.s> N=64.
Ref:	=2006AJ....132.2409N
by	NORRIS R.P. , AFONSO J., APPLETON P.N., BOYLE B.J., CILIEGI P., CROOM S.M., HUYNH M.T., JACKSON C.A., KOEKEMOER A.M., LONSDALE C.J., MIDDELBERG E., MOBASHER B., OLIVER S.J., POLLETTA M., SIANA B.D., SMAIL I., VORONKOV M.A.
	Astron. J., 132, 2409-2423 (2006)
	Deep ATLAS radio observations of the Chandra Deep Field-South/Spitzer wide-area infrared extragalactic field.
o	Table 4: <[NAA2006] CNNN> (Nos C001-C784) = <ATCDFS JHHMMSS.ss+DDMMSS.s> N=784. Table 6: <[NAA2006] SNNN> (Nos S001-S726).
=E=	Catalogue in electronic form as J/AJ/132/2409
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: ATCDFS5
ATCDFS5	(Australia Telescope, ECDFS field, at 5.5GHz) (Not yet in Simbad)
Write:	<<ATCDFS5 JHHMMSS.ss+DDMMSS.s>>
N:	142+212
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ATCA 5.5GHz observations of the extended Chandra Deep Field South, by the Australia Telescope Large Area Survey (ATLAS) team. 2012MNRAS.426.2342H: DR1, N=142 radio sources. 2015MNRAS.454..952H: DR2, N=212 radio sources. See also ATCDFS9.
in source:	NAME ECDFS
Ref:	=2012MNRAS.426.2342H
by	HUYNH M.T. , HOPKINS A.M., LENC E., MAO M.Y., MIDDELBERG E., NORRIS R.P., RANDALL K.E.
	Mon. Not. R. Astron. Soc., 426, 2342-2358 (2012)
	The ATLAS 5.5 GHz survey of the extended Chandra Deep Field South: catalogue, source counts and spectral indices.
o	Table 1, col(1): <[HHL2012] NNN> N=123 among (Nos 1-145), <[HHL2012] NNNA> N=29 among (Nos 31a-31c to 138a-138c). Table 1, col(2): <ATCDFS5 JHHMMSS.ss+DDMMSS.s> N=142.
Ref:	=2015MNRAS.454..952H
by	HUYNH M.T. , BELL M.E., HOPKINS A.M., NORRIS R.P., SEYMOUR N.
	Mon. Not. R. Astron. Soc., 454, 952-972 (2015)
	The ATLAS 5.5 GHz survey of the extended Chandra Deep Field-South: the second data release.
o	Table 2, col(1): <[HBH2015b] NNN> (Nos 1-189), <[HBH2015b] NNN> N=12 among (Nos 20A-20B to 177A-177B). Table 2, col(2): <ATCDFS5 JHHMMSS.ss+DDMMSS.s> N=212.
=E=	Catalogue in electronic form as J/MNRAS/426/2342
=E=	Catalogue in electronic form as <J/MNRAS/454/952/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ATCDFS9
ATCDFS9	(Australia Telescope, ECDFS field, at 9.0GHz)
Write:	<<ATCDFS9 JHHMMSS.ss+DDMMSS.s>>
N:	70
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA 9.0GHz observations of N=70 radio sources in the extended Chandra Deep Field South, by the Australia Telescope Large Area Survey (ATLAS) team. See also ATCDFS5.
in source:	NAME ECDFS
Ref:	=2020MNRAS.491.3395H
by	HUYNH M.T. , SEYMOUR N., NORRIS R.P., GALVIN T.
	Mon. Not. R. Astron. Soc., 491, 3395-3410 (2020)
	The ATLAS 9.0 GHz survey of the extended Chandra Deep Field South: the faint 9.0 GHz radio population.
o	Table 2, col(1): <[HSN2020] NN> N=55 among (Nos 1-70), <[HSN2020] NNA> N=22 among (Nos 14A-14D to 68A-68D). Table 2, col(2): <ATCDFS9 JHHMMSS.ss+DDMMSS.s> N=70.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ATELAIS
ATELAIS	(Australia Telescope, ELAIS field)
Write:	<<ATELAIS JHHMMSS.ss+DDMMSS.s>>
N:	1276
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	The Australia Telescope Large Area Survey (ATLAS) is a project to survey 6 sq deg in the southern sky with the Australia Telescope Compact Array (ATCA). We have conducted 1.4 GHz radio observations with the Australia Telescope Compact Array of an area largely coincident with infrared observations of the Spitzer Wide-Area Extragalactic (SWIRE) Survey, centred on the European Large Area ISO Survey (S1) region. The acronym proposed here is similar to the ATCDFS acronym proposed by Ray Norris, to describe radio sources in the Chandra Deep Field South region, which is part of the ATLAS survey. See also [MNC2008].
in source:	ELAIS S1
Ref:	=2008AJ....135.1276M
by	MIDDELBERG E. , NORRIS R.P., CORNWELL T.J., VORONKOV M.A., SIANA B.D., BOYLE B.J., CILIEGI P., JACKSON C.A., HUYNH M.T., BERTA S., RUBELE S., LONSDALE C.J., IVISON R.J., SMAIL I.
	Astron. J., 135, 1276-1290 (2008)
	Deep Australia Telescope Large Area Survey radio observations of the european large area ISO survey S1/Spitzer wide-area infrared extragalactic field.
o	(Erratum) erratum vol. 136, 519 (2008)
o	PKS 0033-44 not identified.
o	Table 4, col(1): <[MNC2008] CNNNN.N> N=1366 (Nos C1-C1285) = Table 4, col(2): <ATELAIS JHHMMSS.ss+DDMMSS.s> N=1366. Table 5, col(1): <[MNC2008] SNNNN.N>N=1276 among (Nos S1-S1285) = Table 5, col(2): <ATELAIS JHHMMSS.ss+DDMMSS.s> N=1276.
=E=	Catalogue in electronic form as J/AJ/135/1276
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: ATESP
ATESP	(Australia Telescope ESO Slice Project)
Write:	<<ATESP JHHMMSS+DDMMSSA>>
N:	2960
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	The ATESP survey is a radio survey conducted at 1.4 GHz with the Australia Telescope Compact Array on the same region previously covered by the ESO Slice Project redshift survey. The total area covered by the ATESP survey is about 26 sq. deg and the flux limit of the radio-source catalogue extracted is about 0.5 mJy (at 1.4 GHz). Survey is described in 2000A&AS..146...31P
Ref:	=2000A&AS..146...41P
by	PRANDONI I. , GREGORINI L., PARMA P., DE RUITER H.R., VETTOLANI G., WIERINGA M.H., EKERS R.D.
	Astron. Astrophys., Suppl. Ser., 146, 41-55 (2000)
	The ATESP radio survey. II. The source catalogue.
o	<ATESP JHHMMSS+DDMMSSA> N=2960.
=E=	Catalogue in electronic form as VIII/63
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: ATESP5
ATESP5	(Australia Telescope ESO Slice Project, 5GHz)
Write:	<<ATESP5 JHHMMSS+DDMMSSA>>
N:	119
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ATCA 5GHz observations of the region covered by the sub-mJy ATESP survey at 1.4GHz .
Ref:	=2006A&A...457..517P
by	PRANDONI I. , PARMA P., WIERINGA M.H., DE RUITER H.R., GREGORINI L., MIGNANO A., VETTOLANI G., EKERS R.D.
	Astron. Astrophys., 457, 517-529 (2006)
	The ATESP 5 GHz radio survey. I. Source counts and spectral index properties of the faint radio population.
o	Table 6: <ATESP5 JHHMMSS+DDMMSSA> N=119.
=E=	Catalogue in electronic form as J/A+A/457/517
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ATF2003]
[ATF2003]	(Ajiki+Taniguchi+Fujita+, 2003)= (LAE)
Write:	<<[ATF2003] LAE NN>>
N:	20
Object:	LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Suprime-Cam Subaru observations in the field of SDSS J104433.04-012502.2. N=20 LAE candidates. See also [ATM2002], [TAM2003].
Ref:	=2003AJ....126.2091A
by	AJIKI M. , TANIGUCHI Y., FUJITA S.S., SHIOYA Y., NAGAO T., MURAYAMA T., YAMADA S., UMEDA K., KOMIYAMA Y.
	Astron. J., 126, 2091-2107 (2003)
	A SUBARU search for Lyα emitters at redshift 5.7.
o	In the abstract SDSS J104433.04-012522.2 is a misprint for SDSS J104433.04-012502.2.
o	Table 2: <[ATF2003] NN> (Nos 1-20).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ATF2004]
[ATF2004]	(Ajiki+Taniguchi+Fujita+, 2004)
Write:	<<[ATF2004] N>>
N:	4
Object:	LAE (SIMBAD class: EmObj = Emission Object)
Stat:	is completely incorporated in Simbad
Note:	Subaru search for Lyman-alpha emitters. see also [ATF2003].
Ref:	=2004PASJ...56..597A
by	AJIKI M. , TANIGUCHI Y., FUJITA S.S., SHIOYA Y., NAGAO T., MURAYAMA T., YAMADA S.F., UMEDA K., SASAKI S.S., SUMIYA R., KOMIYAMA Y.
	Publ. Astron. Soc. Jap., 56, 597-603 (2004)
	A Subaru search for Lyman-α emitters at z = 5.8 with an intermediate-band filter.
o	In the abstract SDSS J104433.04-012522.2 is a misprint for SDSS J104433.04-012502.2.
o	Table 2: <[ATF2004] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ATH2005]
[ATH2005]	(Apai+Toth+Henning+, 2005)= (NIR)
Write:	<<[ATH2005] IRAS 04381+2540 NIR A>>
N:	2
Object:	(Near IR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Stat:	is completely incorporated in Simbad
Note:	NICMOS image reveals two NIR point sources in IRAS 04381+2540.
in source:	IRAS 04381+2540
Ref:	=2005A&A...433L..33A
by	APAI D. , TOTH L.V., HENNING T., VAVREK R., KOVACS Z., LEMKE D.
	Astron. Astrophys., 433, 33-36 (2005)
	HST/NICMOS observations of a proto-brown dwarf candidate.
o	Fig.1: <[ATH2005] IRAS 04381+2540 NIR A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ATHDFS
ATHDFS	(Australia Telescope, HDFS)
Write:	<<ATHDFS JHHMMSS.s+DDMMSSA>>
N:	87+466+473
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Results from the Australia Telescope HDFS survey. See also [HJN2005] and [HJN2007].
in source:	NAME HDFS
Ref:	=2005AJ....130.1358N
by	NORRIS R.P. , HUYNH M.T., JACKSON C.A., BOYLE B.J., EKERS R.D., MITCHELL D.A., SAULT R.J., WIERINGA M.H., WILLIAMS R.E., HOPKINS A.M., HIGDON J.
	Astron. J., 130, 1358-1372 (2005)
	Radio observations of the Hubble Deep Field-South region. I. Survey description and initial results.
o	Table 3, col(1): numbering 'NN' not used in SIMBAD.
o	Table 3: <ATHDFS JHHMMSS.s+DDMMSSA> N=87.
Ref:	=2005AJ....130.1373H
by	HUYNH M.T. , JACKSON C.A., NORRIS R.P., PRANDONI I.
	Astron. J., 130, 1373-1388 (2005)
	Radio observations of the Hubble Deep Field-South region. II. The 1.4 GHz catalog and source counts.
o	Table 1: <[HJN2005] 1.4GHz NNN> (Nos 1-466) = <ATHDFS JHHMMSS.s+DDMMSSA> N=466.
Ref:	=2007AJ....133.1331H
by	HUYNH M.T. , JACKSON C.A., NORRIS R.P.
	Astron. J., 133, 1331-1344 (2007)
	Radio observations of the Hubble Deep Field-South region. III. The 2.5, 5.2, and 8.7 GHz catalogs and radio source properties.
o	Tables 4, 7: <[HJN2007] 2.5GHz NNN> (Nos 1-149). Tables 5, 8: <[HJN2007] 5.2GHz NN> (Nos 1-42). Tables 6, 9: <[HJN2007] 8.7GHz N> (Nos 1-8). Table 9: <ATHDFS JHHMMSS.s+DDMMSSA> N=463.
=E=	Catalogue in electronic form as J/AJ/130/1373
=E=	Catalogue in electronic form as J/AJ/133/1331
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [ATI98]
[ATI98]	(Artyukh+Tyul'bashev+Isaev, 1998)= (IPS)
Write:	<<[ATI98] HHMMSS+DDMM>>
N:	289
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	See also [AT96]
Ref:	=1998ARep...42..283A
by	ARTYUKH V.S. , TYUL'BASHEV S.A., ISAEV E.A.
	Astron. Rep., 42, 283-292 (1998)
	The cosmological evolution of compact radio sources from 102-MHz observations.
o	1998AZh....75..323A
o	Table 2: <[ATI98] HHMMSS+DDMM> N=289.
=E=	Catalogue in electronic form as VIII/67
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ATK2000]
[ATK2000]	(Aparicio+Tikhonov+Karachentsev, 2000) (Not yet in Simbad)
Write:	<<[ATK2000] NN>>
N:	10
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	N=10 HII regions in DDO 187. Map Fig.5.
in source:	DDO 187
Ref:	=2000AJ....119..177A
by	APARICIO A. , TIKHONOV N., KARACHENTSEV I.
	Astron. J., 119, 177-187 (2000)
	DDO 187: do dwarf galaxies have extended, old halos ?
o	Table 4: <[ATK2000] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ATL2005]
[ATL2005]	(Allam+Tucker+Lee+, 2005)= (CVIG)
Write:	<<[ATL2005] NNNN>>
N:	2980
Object:	G (SIMBAD class: Galaxy)
Note:	New catalog of isolated galaxies from the SDSS DR1.
Ref:	=2005AJ....129.2062A
by	ALLAM S.S. , TUCKER D.L., LEE B.C., SMITH J.A.
	Astron. J., 129, 2062-2073 (2005)
	A catalog of very isolated galaxies from the Sloan Digital Sky Survey data release 1.
o	Table 1: <[ATL2005] NNNN> (Nos 1-2980).
=E=	Catalogue in electronic form as J/AJ/129/2062
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ATL2007]
[ATL2007]	(Allam+Tucker+Lin, 2007)
Write:	<<[ATL2007] LRG>> <<[ATL2007] AN>> <<[ATL2007] Arc>>
N:	1+5+1
Object:	G + Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Stat:	is completely incorporated in Simbad
Note:	Serendipitous discovery of the brightest Lyman Break Galaxy (LBG) currently known (SDSS J002240.78+143113.9) strongly lensed by the Luminous Red Galaxy (LRG) (SDSS J002240.91+143110.4). The LBG is an arc (8 O'Clock arc) which consist of 3 images A1 to A3 and a counterimage A4. The objects B1 is a faint background galaxy.
Ref:	=2007ApJ...662L..51A
by	ALLAM S.S. , TUCKER D.L., LIN H., DIEHL H.T., ANNIS J., BUCKLEY-GEER E.J., FRIEMAN J.A.
	Astrophys. J., 662L, 51-54 (2007)
	The 8 O'Clock arc: a serendipitous discovery of a strongly lensed Lyman break galaxy in the SDSS DR4 imaging data.
o	Fig.1, Table 1: <[ATL2007] LRG> N=1, <[ATL2007] AN> (Nos A1-A4, B1), <[ATL2007] Arc> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ATLAS
ATLAS	(Asteroid Terrestrial-impact Last Alert System)
Write:	<<ATLAS YYaaaa>>
Object:	Transient (SIMBAD class: Transient = Transient Event)
Note:	ATLAS is an asteroid impact early warning system being developed by the University of Hawaii and funded by NASA. It consists of two telescopes, 100 miles apart, which automatically scan the whole sky several times every night looking for moving objects. ATLAS will provide one day's warning for a 30-kiloton "town killer," a week for a 5-megaton "city killer," and three weeks for a 100-megaton "county killer". ATLAS also processes the survey data to search for stationary transients, which are reported to the IAU Transit Name Server. These include supernovae, CVs, stellar outbursts, and fast transients such as GRB afterglows. For more information, visit the project webpage: http://fallingstar.com/ Only the first reference citing ATLAS transients is listed here.
Ref:	=2016ATel.8680....1T
by	TONRY J. , DENNEAU L., STALDER B., HEINZE A., SHERSTYUK A., REST A., SMITH K.W., SMARTT S.J.
	ATel, 8680, 1 (2016)
	Discovery and Classification of 3 Type Supernovae by ATLAS.
o	<NAME ATLAS YYaaa> N=3.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ATLAS
ATLAS	(Australia Telescope Large Area Survey)
Write:	<<ATLAS N JHHMMSS.ss+DDMMSS.sA>> <<ATLAS 3 JHHMMSS.s+DDMMSSC>>
N:	∼15000
Object:	Radio(cm) (SIMBAD class: cmRad = Centimetric Radio Source)
Note:	ATLAS is a deep (∼10 uJy rms) radio survey covering 2 fields around the CDFS-S and ELAIS-S1. Data Release1 took place in 2006-2008 (Norris et al. 2006AJ....132.2409N and Middelberg et al. 2008AJ....135.1276M), and we plan Data Release 2 (Hales et al., to be submitted early 2012) with about 2500 objects and Data Release 3 (Banfield et al., to be submitted late 2012) with about 15000 objects. See also [NAA2006], [MNC2008]. The N in the acronym is the data relase number - either 2 or 3. We will add suffixes to the source designation to indicate individual components or polarisation properties. See http://www.atnf.csiro.au/research/deep/index.html
Ref:	=2014MNRAS.441.2555H
by	HALES C.A. , NORRIS R.P., GAENSLER B.M., MIDDELBERG E., CHOW K.E., HOPKINS A.M., HUYNH M.T., LENC E., MAO M.Y.
	Mon. Not. R. Astron. Soc., 441, 2555-2592 (2014)
	ATLAS 1.4GHz Data Release 2 - I. Observations of the CDF-S and ELAIS-S1 fields and methods for constructing differential number counts.
o	Table A1: <ATLAS2 JHHMMSS.ss+DDMMSS.sA> N=2588. Table B1: <ATLAS2 JHHMMSS.ss+DDMMSS.s> N=2221.
Ref:	=2015MNRAS.453.4020F
by	FRANZEN T.M.O. , BANFIELD J.K., HALES C.A., HOPKINS A., NORRIS R.P., SEYMOUR N., CHOW K.E., HERZOG A., HUYNH M.T., LENC E., MAO M.Y., MIDDELBERG E.
	Mon. Not. R. Astron. Soc., 453, 4020-4036 (2015)
	ATLAS - I. Third release of 1.4 GHz mosaics and component catalogues.
o	Table 5: <ATLAS3 JHHMMSS.s+DDMMSSC> N=5118. ray.norris@csiro.au CSIRO Astronomy & Space Science
=E=	Catalogue in electronic form as <J/MNRAS/441/2555/>
=E=	Catalogue in electronic form as <J/MNRAS/453/4020/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: ATLASGAL
ATLASGAL	(APEX Telescope Large Area Survey of the Galaxy)
*****	Avoid the usage of ATLASGAL, prefer AGAL
Origin	of the Acronym: L = Found in the literature
Details on Acronym: ATLASGAL
ATLASGAL	(APEX Telescope Large Area Survey of the Galaxy)
*****	Avoid the usage of ATLASGAL, prefer [CUS2014]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: ATLBS
ATLBS	(Australia Telescope Low-Brightness Survey)
Write:	<<ATLBS JHHMM.m+DDMMa>>
N:	1094+39+337
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ATCA observations at 1388MHz carried out in two adjacent regions on the sky centred at 00 35 00 -67 00 00 and 00 59 17 -67 00 00 (J2000.0).
Ref:	=2010MNRAS.402.2792S
by	SUBRAHMANYAN R. , EKERS R.D., SARIPALLI L., SADLER E.M.
	Mon. Not. R. Astron. Soc., 402, 2792-2806 (2010)
	ATLBS: the Australia Telescope Low-Brightness Survey.
o	Table 2: <ATLBS JHHMM.m+DDMM> N=1094.
Ref:	=2012ApJS..199...27S
by	SARIPALLI L. , SUBRAHMANYAN R., THORAT K., EKERS R.D., HUNSTEAD R.W., JOHNSTON H.M., SADLER E.M.
	Astrophys. J., Suppl. Ser., 199, 27 (2012)
	ATLBS Extended Source Sample: the evolution in radio source morphology with flux density.
o	Tables 1-2, 4: <ATLBS JHHMM.m+DDMM> N=39 added.
Ref:	=2013ApJ...762...16T
by	THORAT K. , SUBRAHMANYAN R., SARIPALLI L., EKERS R.D.
	Astrophys. J., 762, 16 (2013)
	High-resolution imaging of the ATLBS regions: the radio source counts.
o	Table 2: <ATLBS JHHMM.m+DDMMa> N=337 added.
=E=	Catalogue in electronic form as J/MNRAS/402/2792
=E=	Catalogue in electronic form as J/ApJS/199/27
=E=	Catalogue in electronic form as <J/ApJ/762/16/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ATM2002]
[ATM2002]	(Ajiki+Taniguchi+Murayama+, 2002)= (LAE)
Write:	<<[ATM2002] LAE JHHMM+DDMM>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Suprime-Cam Subaru observations in the field of SDSS J104433.04-012502.2. N=1 new Lyman-Alpha Emitter identified as galaxy. See also [ATF2003], [TAM2003].
Ref:	=2002ApJ...576L..25A
by	AJIKI M. , TANIGUCHI Y., MURAYAMA T., NAGAO T., VEILLEUX S., SHIOYA Y., FUJITA S.S., KAKAZU Y., KOMIYAMA Y., OKAMURA S., SANDERS D.B., OYABU S., KAWARA K., OHYAMA Y., IYE M., KASHIKAWA N., YOSHIDA M., SASAKI T., KOSUGI G., AOKI K., TAKATA T., SAITO Y., KAWABATA K.S., SEKIGUCHI K., OKITA K., SHIMIZU Y., INATA M., EBIZUKA N., OZAWA T., YADOUMARU Y., TAGUCHI H., ANDO H., NISHIMURA T., HAYASHI M., OGASAWARA R., ICHIKAWA S.-I.
	Astrophys. J., 576, 25-28 (2002)
	A new high-redshift Lyα emitter: possible superwind galaxy at z=5.69.
o	<[ATM2002] LAE JHHMM+DDMM> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ATM2009]
[ATM2009]	(Annibali+Tosi+Monelli+, 2009) (Not yet in Simbad)
Write:	<<[ATM2009] NN>>
N:	12
Object:	Poss. Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST (WFPC2 and ACS) observations of NGC 1705.
in source:	NGC 1705
Ref:	=2009AJ....138..169A
by	ANNIBALI F. , TOSI M., MONELLI M., SIRIANNI M., MONTEGRIFFO P., ALOISI A., GREGGIO L.
	Astron. J., 138, 169-183 (2009)
	Young stellar populations and star clusters in NGC 1705.
o	Fig. 5, Table 2: <[ATM2009] NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ATO
ATO	(ATLAS object)= (ATLAS)
Write:	<<ATO JDDD.dddd+DD.ddddA>>
N:	about 500000000
Object:	Unknown (SIMBAD class: Optical = Optical Source)
Note:	The Asteroid Terrestrial-impact Last Alert System (ATLAS, http://fallingstar.com) surveys the entire visible sky four times every two days and collects high quality photometry on all objects brighter than m∼19. We are about to publish light curves of ∼5 million variable stars, submitting data to STScI and Vizier for dissemination. The variability of most of these stars was not previously recognized.
Ref:	=2018AJ....156..241H
by	HEINZE A.N. , TONRY J.L., DENNEAU L., FLEWELLING H., STALDER B., REST A., SMITH K.W., SMARTT S.J., WEILAND H.
	Astron. J., 156, 241-241 (2018)
	A first catalog of variable stars measured by the Asteroid Terrestrial-impact Last Alert System (ATLAS).
o	Table 4 : All objects with Class = MIRA, LPV, PULSE, MPULSE, CBF, CBH, DBF, DBH, SINE, NSINE, MSINE have been ingested in SIMBAD.
o	Table 4: <ATO JDDD.dddd+DD.ddddA> N=4726882. Institute for Astronomy, University of Hawaii
=E=	Catalogue in electronic form as <J/AJ/156/241/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [ATO2015]
[ATO2015]	(Agnello+Treu+Ostrovski+, 2015)
Write:	<<[ATO2015] DES JHHMM+DDMM>> <<[ATO2015] DES JHHMM+DDMM source>> <<[ATO2015] DES JHHMM+DDMM A>> <<[ATO2015] JHHMMSS.s+DDMMSS>>
N:	2+2+6+2
Object:	Grav. lens system + QSO + Grav. lensed image of a QSO + Grav. lens + Pair of G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Magellan 6.5m Baade telescope IMACS spectroscopy of N=2 gravitationally lensed quasars. N=2 pairs of compact, star-forming galaxies. Use of the Dark Energy Survey (DES), Wide-field Infrared Survey Explorer (WISE), and SDSS data.
in source:	DES J0115-5244
in source:	DES J2146-0047
Ref:	=2015MNRAS.454.1260A
by	AGNELLO A. , TREU T., OSTROVSKI F., SCHECHTER P.L., BUCKLEY-GEER E.J., LIN H., AUGER M.W., COURBIN F., FASSNACHT C.D., FRIEMAN J., KUROPATKIN N., MARSHALL P.J., McMAHON R.G., MEYLAN G., MORE A., SUYU S.H., RUSU C.E., FINLEY D., ABBOTT T., ABDALLA F.B., ALLAM S., ANNIS J., BANERJI M., BENOIT-LEVY A., BERTIN E., BROOKS D., BURKE D.L., CARNERO ROSELL A., CARRASCO KIND M., CARRETERO J., CUNHA C.E., D'ANDREA C.B., DA COSTA L.N., DESAI S., DIEHL H.T., DIETRICH J.P., DOEL P., EIFLER T.F., ESTRADA J., NETO A.F., FLAUGHER B., FOSALBA P., GERDES D.W., GRUEN D., GUTIERREZ G., HONSCHEID K., JAMES D.J., KUEHN K., LAHAV O., LIMA M., MAIA M.A.G., MARCH M., MARSHALL J.L., MARTINI P., MELCHIOR P., MILLER C.J., MIQUEL R., NICHOL R.C., OGANDO R., PLAZAS A.A., REIL K., ROMER A.K., ROODMAN A., SAKO M., SANCHEZ E., SANTIAGO B., SCARPINE V., SCHUBNELL M., SEVILLA-NOARBE I., SMITH R.C., SOARES-SANTOS M., SOBREIRA F., SUCHYTA E., SWANSON M.E.C., TARLE G., THALER J., TUCKER D., WALKER A.R., WECHSLER R.H., ZHANG Y.
	Mon. Not. R. Astron. Soc., 454, 1260-1265 (2015)
	Discovery of two gravitationally lensed quasars in the Dark Energy Survey.
o	Fig. 1, Table 1: <[ATO2015] DES JHHMM+DDMM> N=2, <[ATO2015] DES JHHMM+DDMM source> N=2, <[ATO2015] DES JHHMM+DDMM A> N=3+3. Paragr. 3.3: <[ATO2015] JHHMMSS.s+DDMMSS> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ATPMN
ATPMN	(Australia Telescope Compact Array measurements of PMN sources)
Write:	<<ATPMN JHHMMSS.s+DDMMSS>>
N:	∼9000
Object:	(cm) (SIMBAD class: cmRad = Centimetric Radio Source)
Note:	A selection of fields centred on PMN sources observed with the Australia Telescope Compact Array in 1992-1994, but a final catalogue was never published. These data have now been reduced and a catalogue is in preparation; a paper to be sumbitted to MNRAS is in Preparation: "ATPMN: accurate positions and flux densities at 5 and 8 GHz for 8385 PMN sources" by McConnell, D., Sadler, E.M., Murphy, T. and Ekers, R.D.
Auth.:	David McConnell David.McConnell@csiro.au ATNF (CASS), CSIRO
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [ATR2017]
[ATR2017]	(Annibali+Tosi+Romano+, 2017)
Write:	<<[ATR2017] HII-N>> <<[ATR2017] PN-NN>>
N:	6+28
Object:	HII + Poss. PN (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	LBT MODS spectroscopy of N=6 HII regions and N=28 PN candidates, selected on HST ACS images.
in source:	NGC 4449
Ref:	=2017ApJ...843...20A
by	ANNIBALI F. , TOSI M., ROMANO D., BUZZONI A., CUSANO F., FUMANA M., MARCHETTI A., MIGNOLI M., PASQUALI A., ALOISI A.
	Astrophys. J., 843, 20-20 (2017)
	Planetary nebulae and H II regions in the starburst irregular galaxy NGC 4449 from LBT MODS data.
o	Tables 2+5+8: <[ATR2017] HII-N> (Nos HII-1 to HII-6). Tables 3+6+7+9: <[ATR2017] PN-NN> (Nos PN-1 to PN-28).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ATS2000]
[ATS2000]	(Aso+Tatematsu+Sekimoto+, 2000)= (Aso)
Write:	<<[ATS2000] ACNN>>
N:	18
Object:	Core (SIMBAD class: PartofCloud = Part of Cloud)
Note:	N=18 H13CO+ dense cores in OMC 2, OMC3 region.
in source:	OMC:OMC 2 = OMC 2
in source:	OMC:OMC 3 = OMC 3
Ref:	=2000ApJS..131..465A
by	ASO Y. , TATEMATSU K., SEKIMOTO Y., NAKANO T., UMEMOTO T., KOYAMA K., YAMAMOTO S.
	Astrophys. J., Suppl. Ser., 131, 465-482 (2000)
	Dense cores and molecular outflows in the OMC-2/3 region.
o	Table 2: <[ATS2000] ACNN> (Nos AC1-AC18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ATS2004]
[ATS2004]	(Allam+Tucker+Smith+, 2004)
Write:	<<[ATS2004] NNNN>>
N:	1479
Object:	Pair of G (SIMBAD class: PairG = Pair of Galaxies)
Note:	Catalog of merging pair of galaxies in the SDSS EDR.
Ref:	=2004AJ....127.1883A
by	ALLAM S.S. , TUCKER D.L., SMITH J.A., LEE B.C., ANNIS J., LIN H., KARACHENTSEV I.D., LAUBSCHER B.E.
	Astron. J., 127, 1883-1899 (2004)
	Merging galaxies in the Sloan Digital Sky Survey early data release.
o	Table 2: <[ATS2004] NNNN> (Nos 1-1479).
=E=	Catalogue in electronic form as J/AJ/127/1883
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ATW96]
[ATW96]	(Alcala+Terranegra+Wichmann+, 1996)
Write:	<<[ATW96] RX JHHMM.m+DDMMa>>
N:	4
Object:	T Tau * (SIMBAD class: TTauri* = T Tauri Star)
Stat:	is completely incorporated in Simbad
Note:	N=4 WTTS, possible optical counterpart of the corresponding RX J See also [AKS95b], [WKS96], [CAA97], [MMS97], [KWS97], [WSK97], [HMC99].
Ref:	=1996A&AS..119....7A
by	ALCALA J.M. , TERRANEGRA L., WICHMANN R., CHAVARRIA-K. C., KRAUTTER J., SCHMITT J.H.M.M., MORENO-CORRAL M.A., DE LARA E., WAGNER R.M.
	Astron. Astrophys., Suppl. Ser., 119, 7-24 (1996)
	New weak-line T Tauri stars in Orion from the ROSAT all-sky survey.
o	Table 3: <[ATW96] RX JHHMM.m+DDMMa> N=4
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ATZ98]
[ATZ98]	(Appenzeller+Thiering+Zickgraf+, 1998)
Write:	<<[ATZ98] ANNN>> <<[ATZ98] JHHMMSS.s+DDMMSS>>
N:	674+70+16
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT All-Sky-Survey (RASS) sources, format 'ANNN', letter 'A' stands for fields (Nos A-F) In remarks, N=16 objects are identified by their J2000 coord., 'JHHMMSS.s+DDMMSS' in the fields of some X.
Ref:	=1998ApJS..117..319A
by	APPENZELLER I. , THIERING I., ZICKGRAF F.-J., KRAUTTER J., VOGES W., CHAVARRIA C., KNEER R., MUJICA R., PAKULL M., ROSSO C., RUZICKA F., SERRANO A., ZIEGLER B.
	Astrophys. J., Suppl. Ser., 117, 319-340 (1998)
	Identification of a complete sample of northern ROSAT all-sky survey X-ray sources. III. The catalog.
o	(Erratum) Erratum vol. 134, p. 179 (2001)
o	Table 1: <[ATZ98] ANNN> N=744 among (Nos A001-A161, B001-B209, C001-C203, D001-D153, E001-E265, F001-F142). Remarks: <[ATZ98] JHHMMSS.s+DDMMSS> N=16.
=E=	Catalogue in electronic form as J/ApJS/117/319
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AU
AU	(Auriere+)
*****	Avoid the usage of AU, prefer ACH
Origin	of the Acronym: L (2007A&A...471..127G)
Details on Acronym: [AU88]
[AU88]	(Antonucci+Ulvestad, 1988)
Write:	<<[AU88] S.sss-SS.ss>> <<[AU88] S.ss-SS.s>>
N:	64
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=64 compact radio-sources in NGC 253. Format: offset relative to RA = 00h45m, Dec = -25deg33' (1950). See also [LT2006b].
in source:	NGC 253
Ref:	=1988ApJ...330L..97A
by	ANTONUCCI R.R.J. , ULVESTAD J.S.
	Astrophys. J., 330, 97-100 (1988)
	A large family of compact radio sources in the starburst nucleus of NGC 253.
o	Table 1: <[AU88] S.sss-SS.ss> N=35
Ref:	=1991AJ....102..875U
by	ULVESTAD J.S. , ANTONUCCI R.R.J.
	Astron. J., 102, 875-881 (1991)
	Second-epoch VLA observations of compact radio sources in NGC 253.
o	Table 1: <[AU88] S.sss-SS.ss> N=42, 7 new
Ref:	=1994ApJ...424L..29U
by	ULVESTAD J.S. , ANTONUCCI R.R.J.
	Astrophys. J., 424, 29-32 (1994)
	Do the compact radio sources in NGC 253 and M 82 fade over time ?
o	Table 1: <[AU88] S.ss-SS.s> N=11
Ref:	=1997ApJ...488..621U
by	ULVESTAD J.S. , ANTONUCCI R.R.J.
	Astrophys. J., 488, 621-641 (1997)
	VLA observations of NGC 253: supernova remnants and H II regions at 1 parsec resolution.
o	Table 12: <[AU88] S.ss-SS.s> N=64
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AUD2007]
[AUD2007]	(Adami+Ulmer+Durret+, 2007)
Write:	<<[AUD2007] Cl JHHMM+DDMM>> <<[AUD2007] ClJHHMM+DDMM>> (not recognised by Simbad, but found in literature)
N:	37
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Search for distant clusters of galaxies based on optical and X-ray candidates from the SHARC survey.
Ref:	=2007A&A...472..373A
by	ADAMI C. , ULMER M.P., DURRET F., COVONE G., CYPRIANO E., HOLDEN B.P., KRON R., LIMA NETO G.B., ROMER A.K., RUSSEIL D., WILHITE B.
	Astron. Astrophys., 472, 373-381 (2007)
	An extension of the SHARC survey.
o	Table 1: <[AUD2007] Cl JHHMM+DDMM> N=37.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AUDS
AUDS	(HI Arecibo Ultra-Deep Survey)
Write:	<<AUDS NNN>> <<AUDS JHHMMSS+DDMMSS>>
N:	247
Object:	G (SIMBAD class: Galaxy)
Note:	HI Arecibo Ultra-Deep Survey (AUDS) is a deep blind 21 cm line survey of two selected fields carried out with the Arecibo radio telescope to detect N=247 galaxies at redshifts between 0 and 0.16 2011ApJ...727...40F is the first ref. N=18 galaxies. See [FSC2011]. 2015MNRAS.452.3726H correspond to 60 per cent of the total survey with the format JHHMMSS+DDMMSS. N=102 galaxies 2021MNRAS.501.4550X is the final survey with the format 'NNN'. N=247 galaxies.
Ref:	=2015MNRAS.452.3726H
by	HOPPMANN L. , STAVELEY-SMITH L., FREUDLING W., ZWAAN M.A., MINCHIN R.F., CALABRETTA M.R.
	Mon. Not. R. Astron. Soc., 452, 3726-3741 (2015)
	A blind HI mass function from the Arecibo Ultra-Deep Survey (AUDS).
o	Table A1: <AUDS JHHMMSS+DDMMSS> N=102.
Ref:	=2021MNRAS.501.4550X
by	XI H. , STAVELEY-SMITH L., FOR B.-Q., FREUDLING W., ZWAAN M., HOPPMANN L., LIANG F.-H., PENG B.
	Mon. Not. R. Astron. Soc., 501, 4550-4564 (2021)
	The Arecibo Ultra-Deep Survey.
o	Table 2: <AUDS NNN> (Nos 1-247).
=E=	Catalogue in electronic form as <J/MNRAS/501/4550/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AUK96]
[AUK96]	(Awaki+Ueno+Koyama+, 1996) (Not yet in Simbad)
Write:	<<[AUK96] A>>
N:	4
Object:	(X) (SIMBAD class: X = X-ray Source)
in source:	NGC 1808
Ref:	=1996PASJ...48..409A
by	AWAKI H. , UENO S., KOYAMA K., TSURU T., IWASAWA K.
	Publ. Astron. Soc. Jap., 48, 409-416 (1996)
	ASCA observation of NGC 1808.
o	T.5: obj. are in Simbad as '[JZH95] NN' (last col.)
o	Table 5: <[AUK96] A> (Nos A-D)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AUO2003]
[AUO2003]	(Akiyama+Ueda+Ohta+, 2003)
Write:	<<[AUO2003] JHHMMSS.ss+DDMMSS.s>>
N:	132
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	ASCA Medium Sensitivity Survey in the Northern sky: Search for optical identification of 87 hard 1AXG X-ray sources.
Ref:	=2003ApJS..148..275A
by	AKIYAMA M. , UEDA Y., OHTA K., TAKAHASHI T., YAMADA T.
	Astrophys. J., Suppl. Ser., 148, 275-315 (2003)
	Optical identification of the ASCA medium sensitivity survey in the northern sky: nature of hard X-Ray-Selected luminous active galactic nuclei.
o	Table 1, col(2): Identification number AANN (AA = NO, NE, SE) represents the number of a source in three source lists used during the optical identification observations, not used in SIMBAD.
o	Table 1: <[AUO2003] JHHMMSS.ss+DDMMSS.s> N=132.
=E=	Catalogue in electronic form as J/ApJS/148/275
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Aur
Aur	(Auriga)
*****	Avoid the usage of Aur, prefer [MWC53]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Av
Av	(Antalova)
*****	Avoid the usage of Av, prefer Antalova
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AV
AV	(Azzopardi+Vigneau+)
====>	Equivalent to: AzV
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Av-Hunter
Av-Hunter	= Aveni-Hunter (Not yet in Simbad)
Write:	<<Av-Hunter N>>
N:	1
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Details on Acronym: [AV96]
[AV96]	(Andreazza+Vilas-Boas, 1996)
Write:	<<[AV96] Lupus N A>>
N:	17
Object:	Condensation (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Condensations in 4 clouds: In Lupus 1: N=6 condensations (Nos A-F) In Lupus 2: N=3 condensations (Nos A-C) In Lupus 3: N=4 condensations (Nos A-D) In Lupus 4: N=4 condensations (Nos A-D)
in source:	NAME Lupus Cloud
in source:	NAME Lupus I = Lupus 1
in source:	NAME Lupus II = Lupus 2
in source:	NAME Lupus III = Lupus 3
in source:	NAME Lupus IV = Lupus 4
Ref:	=1996A&AS..116...21A
by	ANDREAZZA C.M. , VILAS-BOAS J.W.S.
	Astron. Astrophys., Suppl. Ser., 116, 21-30 (1996)
	Star counts in southern dark clouds: Corona Australis and Lupus.
o	Table 7: <[R78] Cloud A> No. F is new. Table 7: <[AV96] Lupus 1 A> (Nos A-C), <[AV96] Lupus 2 A> (Nos A-D), <[AV96] Lupus 3 A> (Nos A-D), <[AV96] Lupus 4 A> (Nos A-F).
=E=	Catalogue in electronic form as J/A+AS/116/21
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AVB2002]
[AVB2002]	(Alexander+Vignali+Bauer+, 2002)
Write:	<<[AVB2002] JHHMMSS.ss+DDMMSS.s>>
N:	29+9+13
Object:	Very Red Object (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of VRO in the CDFN.
in source:	NAME CDFN
Ref:	=2002AJ....123.1149A
by	ALEXANDER D.M. , VIGNALI C., BAUER F.E., BRANDT W.N., HORNSCHEMEIER A.E., GARMIRE G.P., SCHNEIDER D.P.
	Astron. J., 123, 1149-1162 (2002)
	The Chandra Deep Field North survey. X. X-ray emission from very red objects.
o	Tables 2 to 4: <[AVB2002] JHHMMSS.ss+DDMMSS.s> N=29+9+13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AVC
AVC	(Anomalous Velocity Cloud) (Not yet in Simbad)
*****	Avoid the usage of AVC, prefer [MBW2009]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AVD90]
[AVD90]	(Afanasiev+Vlasyuk+Dodonov+, 1990)= ([AVD90a])
Write:	<<[AVD90] NNNN>>
N:	2222 among 9168
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Ref:	=1990AISAO..32...73A
by	AFANASIEV V.L. , VLASYUK V.V., DODONOV S.N., SPIRIDONOVA O.N., RICHTER G., NOVIKOV S.B., BUGAENKO O.I., SHOKIN Y.A., SHUL'GA V.V.
	Astrofizik. Issledovanija, 32, 73-105 (1990)
	Photometrical investigation of the complete up to B=21m sample of objects in the field 9h40m +50.
o	Table 3a not in Simbad
o	Table 3: <[AVD90] NNNN> N=2222 among 9168
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AVD90a]
[AVD90a]	(Afanasiev+Vlasyuk+Dodonov+, 1990)
*****	Avoid the usage of [AVD90a], prefer [AVD90]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AVD90b]
[AVD90b]	(Afanasiev+Vlasyuk+Dodonov+, 1990)= (M82)
Write:	<<[AVD90b] SA 68 NNN>> <<[AVD90b] M 82 NNN>> <<[AVD90b] SA 57 NNN>>
N:	150+138+230
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	In SIMBAD, we use the numbering Nf in the col.(2), as used in Veron+,1996. Table 3: objects in SA 68, N=150 among (Nos 1-177) Table 4: objects in M 83, N=138 among (Nos 1-162) Table 5: objects in SA 57, N=230 among (Nos 1-512)
Ref:	=1990AISAO..32...31A
by	AFANASIEV V.L. , VLASYUK V.V., DODONOV S.N., LORENZ H., TEREBIZH V.Y.
	Astrofizik. Issledovanija, 32, 31-65 (1990)
	Spectral and photometrical investigation of objects in selected fields with the 6-m telescope.
o	Tables 3-5: don't use the running number in 1st col., but the numbering Nf in col.(2)
o	Table 3: <[AVD90b] SA 68 NNN> N=150 among (Nos 1-177). Table 4: <[AVD90b] M 82 NNN> N=138 among (Nos 1-162). Table 5: <[AVD90b] SA 57 NNN> N=230 among (Nos 1-512).
=E=	Catalogue in electronic form as J/other/AISAO/32.31
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AVE98]
[AVE98]	(Anglada+Villuendas+Estalella+, 1998)= (VLA)
Write:	<<[AVE98] LDN NNNNA N>> <<[AVE98] Haro 4-255 N>> <<[AVE98] HH 24-26 NN>>
N:	37
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Continuum radio-sources in the field of 6 YSO. See also [ARC92], [BAW95].
Ref:	=1998AJ....116.2953A
by	ANGLADA G. , VILLUENDAS E., ESTALELLA R., BELTRAN M.T., RODRIGUEZ L.F., TORRELLES J.M., CURIEL S.
	Astron. J., 116, 2953-2964 (1998)
	Spectral indices of centimeter continuum sources in star-forming regions: implications on the nature of the outflow exciting sources.
o	* SSV 61 = SSV LDN 1630 61. T.2: sources in RNO 43 = [ARC92] RNO 43 N.
o	Table 2: <[ARC92] AS 353A N> (Nos 6-8) added, <[ARC92] Barn 335 NN> (Nos 8-12) added. Table 2: <[AVE98] LDN 1641N N> (Nos 1-7), <[AVE98] Haro 4-255 N> (Nos 1-2), <[AVE98] HH 24-26 NN> (Nos 1-11), <[AVE98] LDN 1617 N> (Nos 1-8), <[AVE98] LDN 1251B N> (Nos 1-4), <[AVE98] LDN 1262 N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Aveni-Hunter
Aveni-Hunter	(Aveni+Hunter)
*****	Avoid the usage of Aveni-Hunter, prefer AH
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Aveni-Hunter
Aveni-Hunter	(Aveni+Hunter)
Write:	<<NAME AVENI-HUNTER N>>
N:	1
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Stat:	is completely incorporated in Simbad
Ref:	=1969AJ.....74.1021A
by	AVENI A.F. , HUNTER J.H.
	Astron. J., 74, 1021-None (1969)
	Observational studies relating to star formation. II.
o	<Cl AH 1> = <NAME AVENI-HUNTER 1>.
Details on Acronym: [AVG2008]
[AVG2008]	(Anandarao+Venkata Raman+Ghosh+, 2008)
Write:	<<[AVG2008] Cluster NW>> <<[AVG2008] Star A>> <<[AVG2008] Cluster NW NN>> <<[AVG2008] JHHMMSS.ss+DDMMSS.ss>>
N:	3+1+12+13+12+86+62+30
Object:	Cluster of * + * + TT* + NIR (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	UKIRT near-infrared photometry of the massive star-forming regions IRAS 21413+5442 and IRAS 21407+5441.
Ref:	=2008MNRAS.390.1185A
by	ANANDARAO B.G. , VENKATA RAMAN V., GHOSH S.K., OJHA D.K., KUMAR M.S.N.
	Mon. Not. R. Astron. Soc., 390, 1185-1194 (2008)
	Near-infrared photometry and radio continuum study of the massive star-forming regions IRAS 21413+5442 and IRAS 21407+5441.
o	Star A = 2MASS J21424319+5455519
o	Fig. 1: <[AVG2008] Cluster NW> (Nos 1, 2C, 2N), <[AVG2008] Star A> (No. A). Tables 1, 2, 3: <[AVG2008] JHHMMSS.ss+DDMMSS.ss> N=86+62+30. Fig. 2, Table 1, col(6): <[AVG2008] Cluster 1 NN> (Nos 1-12). Fig.3, Table 1, col(6): <[AVG2008] Cluster 2C NN> (Nos 1-13). Fig.2, Table 1, col(6): <[AVG2008] Cluster 2N NN> (Nos 1-12).
=E=	Catalogue in electronic form as J/MNRAS/390/1185
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AVG96]
[AVG96]	(Abraham+Van Den Bergh+Glazebrook+, 1996)= (MDS)
Write:	<<[AVG96] ua-0-NN>> <<[AVG96] aaNN-NNN>> <<[AVG96] aaaN-NNN>> <<[AVG96] uNaN-NNN>>
N:	508+395
Object:	G (SIMBAD class: Galaxy)
Note:	HST MDS survey of high redshift galaxies. The format is the MDS (Medium Deep Survey) identity, first part for the MDS field, second part 'NN' for each galaxy within the field. [TSM2001] and [YT2003] also used the HST-MDS identity.
Ref:	=1996ApJS..107....1A
by	ABRAHAM R.G. , VAN DEN BERGH S., GLAZEBROOK K., ELLIS R.S., SANTIAGO B.X., SURMA P., GRIFFITHS R.E.
	Astrophys. J., Suppl. Ser., 107, 1-17 (1996)
	The morphologies of distant galaxies. II. Classifications from the Hubble space telescope medium deep survey.
o	Table 1: <[AVG96] ua-0-NN>, <[AVG96] aaNN-NNN>, <[AVG96] aaaN-NNN> N=508
Ref:	=1998MNRAS.297..885G
by	GLAZEBROOK K. , ABRAHAM R., SANTIAGO B., ELLIS R., GRIFFITHS R.
	Mon. Not. R. Astron. Soc., 297, 885-904 (1998)
	The physical parameters of the evolving population of faint galaxies.
o	Table 2: <[AVG96] ua-0-NN>, <[AVG96] aaNN-NNN>, <[AVG96] aaaN-NNN>, <[AVG96] uNaN-NNN> N=395 new.
=E=	Catalogue in electronic form as J/MNRAS/297/885
=E=	Catalogue in electronic form as J/ApJS/107/1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AVL99]
[AVL99]	(Alonso+Valotto+Lambas+, 1999)
Write:	<<[AVL99] JHHMMSS.s+DDMMSS.s>>
N:	83
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=83 galaxies in 18 ClG.
Ref:	=1999MNRAS.308..618A
by	ALONSO M.V. , VALOTTO C., LAMBAS D.G., MURIEL H.
	Mon. Not. R. Astron. Soc., 308, 618-622 (1999)
	Velocity dispersion estimates of APM galaxy clusters.
o	Table 3: <[AVL99] JHHMMSS.s+DDMMSS.s> N=83.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AVN2003]
[AVN2003]	(Abraham+Van den Bergh+Nair, 2003)
Write:	<<[AVN2003] NNNNNN-NN-N-NNNN-NNNN>>
N:	930
Object:	G (SIMBAD class: Galaxy)
Note:	SDSS EDR statistics for quantifying galaxy morphology. The SDSS format stands for 'Run-Rerun-Camcol-Field-ID'.
Ref:	=2003ApJ...588..218A
by	ABRAHAM R.G. , VAN DEN BERGH S., NAIR P.
	Astrophys. J., 588, 218-229 (2003)
	A new approach to galaxy morphology. I. Analysis of the Sloan Digital Sky Survey early data release.
o	Table 1: <[AVN2003] NNNNNN-NN-N-NNNN-NNNN> N=930.
=E=	Catalogue in electronic form as J/ApJ/588/218
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AVS2017]
[AVS2017]	(Allen+Van Der Tak+Sanchez-Monge+, 2017)
Write:	<<[AVS2017] G35.20AN>>
N:	4
Object:	Core (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Notes:	ALMA Cycle 0 band 7 observations of N=4 cores toward the high-mass star-forming region G35.20-0.74N. See also [BSC2014].
in source:	NAME G 35.2-0.74N
Ref:	=2017A&A...603A.133A
by	ALLEN V. , VAN DER TAK F.F.S., SANCHEZ-MONGE A., CESARONI R., BELTRAN M.T.
	Astron. Astrophys., 603A, 133-133 (2017)
	Chemical segregation in hot cores with disk candidates. An investigation with ALMA.
o	Tables 1-3, Fig. 1: <[AVS2017] G35.20AN> (Nos A, B1-B3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AW2003]
[AW2003]	(Angelini+White, 2003)
Write:	<<[AW2003] N>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observation of 4U 1755-33 field. N=3 sources.
Ref:	=2003ApJ...586L..71A
by	ANGELINI L. , WHITE N.E.
	Astrophys. J., 586, 71-75 (2003)
	An XMM-Newton observation of 4U 1755-33 in quiescence: evidence of a fossil X-ray jet.
o	Table 2: <[AW2003] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AW90]
[AW90]	(Aspin+Walther, 1990)= (IRS)
Write:	<<[AW90] a>> <<[AW90] ai>> <<[AW90] aii>> <<[AW90] aWW>>
N:	17
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Point-like source in Mon R2. 1st ref.: (Nos ai, aii, b-h) 2nd ref.: (Nos aN, aS, bN, bS, cN, cS, dN, dS) are added
in source:	NAME Mon R2 GMC
Ref:	=1990A&A...235..387A
by	ASPIN C. , WALTHER D.M.
	Astron. Astrophys., 235, 387-394 (1990)
	Infrared imaging polarimetry of Monoceros R2 IRS.
o	Table 1: <[BEB76] IRS 1a>. Table 1: <[AW90] aii> (Nos ai, aii, b-h)
Ref:	=1994ApJ...425..707H
by	HOWARD E.M. , PIPHER J.L., FORREST W.J.
	Astrophys. J., 425, 707-719 (1994)
	A near-infrared study of the Monoceros R2 star formation region.
o	Table 2: <[AW90] aW> (Nos aN, aS, bN, bS, cN, cS, dN, dS) added. Table 2: <[BEB76] IRS NWW> (Nos 1NE, 1SW, 4N, 4S, 5N, 5S, 9) added
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AWA2011]
[AWA2011]	(Aretxaga+Wilson+Aguilar+, 2011)= (AzTEC/C) = (AzTEC)
Write:	<<[AWA2011] AzTEC/CNNN>>
N:	189
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ASTE AzTEC observations in the COSMOS field. See also AzTEC.
in source:	NAME COSMOS Field
Ref:	=2011MNRAS.415.3831A
by	ARETXAGA I. , WILSON G.W., AGUILAR E., ALBERTS S., SCOTT K.S., SCOVILLE N., YUN M.S., AUSTERMANN J., DOWNES T.P., EZAWA H., HATSUKADE B., HUGHES D.H., KAWABE R., KOHNO K., OSHIMA T., PERERA T.A., TAMURA Y., ZEBALLOS M.
	Mon. Not. R. Astron. Soc., 415, 3831-3850 (2011)
	AzTEC millimetre survey of the COSMOS field – III. Source catalogue over 0.72 °^{2} and plausible boosting by large-scale structure.
o	(Erratum) erratum vol. 419, p. 1824 (2012)
o	Table 1, col(1): <[AWA2011] AzTEC/CNNN> (Nos 1-189) = Table 1, col(2): <AzTEC JHHMMSS.ss+DDMMSS.s> N=189.
=E=	Catalogue in electronic form as <J/MNRAS/415/3831/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AWA90]
[AWA90]	(Alvarado+Wenderoth+Alcaino+, 1990)
Write:	<<[AWA90] NGC 6752 A>> <<[AWA90] NGC 6864 A>>
N:	13+7
Object:	Star (SIMBAD class: Star)
Note:	La Silla 1m UBVRI photoelectric observations of N=13+7 stars in the Galactic globular clusters NGC 6752 and NGC 6864.
in source:	NGC 6752
in source:	NGC 6864
Ref:	=1990AJ.....99.1501A
by	ALVARADO F. , WENDEROTH E., ALCAINO G., LILLER W.
	Astron. J., 99, 1501-1503 (1990)
	Photoelectric UBVRI sequences in the galactic globular clusters NGC 6752 and NGC 6864.
o	Table IV: <[AWA90] NGC 6752 A> (Nos A-M), Table V: <[AWA90] NGC 6864 A> (Nos A-G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AWC2004]
[AWC2004]	(Alcala+Wachter+Covino+, 2004)
Write:	<<[AWC2004] TTS JHHMMSS.s+DDMMSS>> <<[AWC2004] RX J0506.9-0319 WW>> <<[AWC2004] RX J0506.9-0320 W>> <<[AWC2004] RX J0506.4-0328 W>>
N:	28+6
Object:	PMS* (SIMBAD class: YSO = Young Stellar Object)
Note:	Multi-wavelength observations of the star forming region LDN 1616 including ROSAT RASS and HRI observations. TTau* (TTS in the format) and part of RX sources.
in source:	LDN 1616
Ref:	=2004A&A...416..677A
by	ALCALA J.M. , WACHTER S., COVINO E., STERZIK M.F., DURISEN R.H., FREYBERG M.J., HOARD D.W., COOKSEY K.
	Astron. Astrophys., 416, 677-697 (2004)
	Multi-wavelength observations of the star forming region in L1616.
o	Table 3: <[AWC2004] TTS JHHMMSS.s+DDMMSS> N=7, <[AWC2004] RX J0506.9-0319 WW> (Nos SE, NW), <[AWC2004] RX J0506.9-0320 W> (Nos W, E). Table A1: <[AWC2004] RX J0506.4-0328 W> (Nos W, E).
Ref:	=2008ApJ...687.1303G
by	GANDOLFI D. , ALCALA J.M., LECCIA S., FRASCA A., SPEZZI L., COVINO E., TESTI L., MARILLI E., KAINULAINEN J.
	Astrophys. J., 687, 1303-1322 (2008)
	The star formation in the L1615/L1616 cometary cloud.
o	Table 2: <[AWC2004] TTS JHHMMSS.s+DDMMSS> N=21 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AWC2015]
[AWC2015]	(Ansdell+Williams+Cieza+, 2015) (Not yet in Simbad)
Write:	<<[AWC2015] SMG JHHMMSS.s+DDMMSS>>
N:	3
Object:	Poss. smm G (SIMBAD class: Galaxy)
Note:	JCMT SCUBA-2 850µm observations of N=3 candidate sub-mm galaxies (SMGs) in the field of the λ Orionis Cluster.
in source:	NAME lam Ori Cluster
Ref:	=2015ApJ...806..221A
by	ANSDELL M. , WILLIAMS J.P., CIEZA L.A.
	Astrophys. J., 806, 221 (2015)
	A SCUBA-2 850-micron survey of circumstellar disks in the λ Orionis cluster.
o	Table 4: <[AWC2015] SMG JHHMMSS.s+DDMMSS> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AWH84]
[AWH84]	(Arp+Wolstencroft+He+, 1984)
Write:	<<[AWH84] NGC 1097 NN>>
N:	43
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Note:	Poss. QSOs near NGC 1097. See Paper I: [WKA83]
Ref:	=1984ApJ...285...44A
by	ARP H. , WOLSTENCROFT R.D., HE X.T.
	Astrophys. J., 285, 44-54 (1984)
	Complete quasar search in the NGC 1097 field.
o	Table 2: <[AWH84] NGC 1097 NN> (Nos 1-43).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AWK2020]
[AWK2020]	(Abdullah+Wilson+Klypin+, 2020)
Write:	<<[AWK2020] NNNN>>
N:	1800
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=1800 galaxy clusters, identified from SDSS DR13 spectroscopic data.
Ref:	=2020ApJS..246....2A
by	ABDULLAH M.H. , WILSON G., KLYPIN A., OLD L., PRATON E., ALI G.B.
	Astrophys. J., Suppl. Ser., 246, 2-2 (2020)
	GalWeight application: a publicly available catalog of dynamical parameters of 1800 galaxy clusters from SDSS-DR13, (GalWCat19).
o	galwcls.dat: <[AWK2020] NNNN> (Nos 1-1800).
=E=	Catalogue in electronic form as <J/ApJS/246/2/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AWM
AWM	(Albert+White+Morgan)
Write:	<<AWM N-NN>>
N:	31
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Ref:	=1977ApJ...211..309A
by	ALBERT C.E. , WHITE R.A., MORGAN W.W.
	Astrophys. J., 211, 309-310 (1977)
	cD galaxies in poor clusters. II.
o	Table 1: <AWM N> (Nos 1-7). Table 2: <AWM 1-N> (Nos 1, 2), <AWM 2-N> (Nos 1, 5, 7), <AWM 3-N> (Nos 1, 5), <AWM 4-N> (Nos 1, 5, 6), <AWM 5-N> (No. 6), <AWM 6-N> (Nos 1, 2), <AWM 7-N> (No. 1).
Ref:	=1980ApJ...235..347S
by	STAUFFER J. , SPINRAD H.
	Astrophys. J., 235, 347-350 (1980)
	Redshifts for galaxies in three Yerkes poor clusters.
o	Table 1: <AWM 7-NN> (Nos 1 to 13), <AWM 1-N> (Nos 1, 2), <AWM 5-N> (Nos 1 to 5).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AWM
AWM	(Albert+White+Morgan)
Write:	<<AWM N>>
N:	7
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Paper I: MKW
Ref:	=1977ApJ...211..309A
by	ALBERT C.E. , WHITE R.A., MORGAN W.W.
	Astrophys. J., 211, 309-310 (1977)
	cD galaxies in poor clusters. II.
o	Table 1: <AWM N> (Nos 1-7). Table 2: <AWM 1-N> (Nos 1, 2), <AWM 2-N> (Nos 1, 5, 7), <AWM 3-N> (Nos 1, 5), <AWM 4-N> (Nos 1, 5, 6), <AWM 5-N> (No. 6), <AWM 6-N> (Nos 1, 2), <AWM 7-N> (No. 1).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [AWM2000]
[AWM2000]	(Andersson+Wannier+Moriarty-Scheven+, 2000)
Write:	<<[AWM2000] 1-NNA>> <<[AWM2000] 2-NNA>>
N:	16+17
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Penticton observations. Radio continuum sources: Table 1: at 408MHz, format '1-NNA'. Table 2: at 1420MHz, format '2-NNA'.
in source:	NAME Per Region
Ref:	=2000AJ....119.1325A
by	ANDERSSON B.-G. , WANNIER P.G., MORIARTY-SCHIEVEN G.H., BAKKER E.J.
	Astron. J., 119, 1325-1338 (2000)
	The nature of the IRAS ring G159.6-18.5 in Perseus and its exciting star HD 278942.
o	Table 1: <[AWM2000] 1-NNA> (Nos 1-13, 16, 16A-16B). Table 2: <[AWM2000] 2-NNA> (Nos 1-12, 1A-1B, 8A-8C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AWP2011]
[AWP2011]	(Aravena+Wagg+Papadopoulos+, 2011)
Write:	<<[AWP2011] H1821+643 companion>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	CARMA 12CO(1-0) observations of the field of H1821+643.
Ref:	=2011ApJ...737...64A
by	ARAVENA M. , WAGG J., PAPADOPOULOS P.P., FEAIN I.J.
	Astrophys. J., 737, 64 (2011)
	Unveiling the mask on the ULIRG-to-QSO transition object [H89]1821+643 at z = 0.3: a gas-poor/gas-rich galaxy merger and the implications for co-based dynamical mass estimates.
o	Table 1: <[AWP2011] H1821+643 companion> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AWW90]
[AWW90]	(Assendorp+Wesselius+Whittet+, 1990)= (IRS)
Write:	<<[AWW90] Ced 111 IRS N>> <<[AWW90] Ced 112 IRS N>>
N:	7+8
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	High resolution IRAS pointed observations. See also: Ass Cha T, WKK, [PCW91].
in source:	Ced 111
in source:	Ced 112
Ref:	=1990MNRAS.247..624A
by	ASSENDORP R. , WESSELIUS P.R., WHITTET D.C.B., PRUSTI T.
	Mon. Not. R. Astron. Soc., 247, 624-631 (1990)
	A study of the Chamaeleon I dark cloud and T-association. II. High-resolution IRAS maps around HD 97048 and 97300.
o	Cross-id: IRAS, TNN = Ass Cha T 2-NN, C N-NN et E N-NN = HJM C N-NN et HJM E N-NN, FNN = WKK FNN.
o	Table 2: <[AWW90] Ced 111 IRS N> (Nos 1-7), <[AWW90] Ced 112 IRS N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AX
AX	(ASCA satellite, X-ray)= AXS
Write:	<<AX HHMM.m+DDMM>> <<AX JHHMM.m+DDMM>> <<AX JHHMM+DDd>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	First references from the ASCA satellite survey. In each ref., N=1 soft X-ray, with a 1950 coord. format or a 2000 coord. format.
Ref:	=1994Natur.368..127M
by	MURAKAMI T. , TANAKA Y., KULKARNI S.R., OGASAKA Y., SONOBE T., OGAWARA Y., AOKI T., YOSHIDA A.
	Nature, 368, 127-129 (1994)
	X-ray identification of the soft γ-ray repeater 1806-20.
o	First ref. from the ASCA satellite survey. In this ref. <AX HHMM.m+DDMM> N=1
Ref:	=1995PASJ...47..189Y
by	YAMAUCHI S. , AOKI T., HAYASHIDA K., KANEDA H., KOYAMA K., SUGIZAKI M., TANAKA Y., TOMIDA H., TSUBOI Y.
	Publ. Astron. Soc. Jap., 47, 189-194 (1995)
	New transient X-ray source in the Scutum region discovered with ASCA.
o	<AX JHHMM.m+DDMM> first reference from the ASCA satellite survey with this format, N=1
Ref:	=1995IAUC.6260....1M
by	MISAKI K. , KAMATA Y., TERASHIMA Y., IMSOBE K., KUNIEDA H., TAWARA Y., TAURU T., MAEDA Y., SAKANO M., AKIYAMA M., SOGAWA H., ISHIDA M., FUJIMOTO R.
	IAU Circ., 6260, 1-None (1995)
	AX J2315-592.
o	<AX JHHMM+DDd> first reference from the ASCA satellite survey with this format, N=1
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 1AXG
1AXG	(1st ASCA X-ray survey, GIS)
Write:	<<1AXG JHHMMSS+DDMM>>
N:	1343+1190
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	First (AMSS-I) and second (AMSS-II) X-ray source catalogs (ASCA Medium Sensitivity Survey), from GIS experiment (Gas Imaging Spectrometer).
Ref:	=2001ApJS..133....1U
by	UEDA Y. , ISHISAKI Y., TAKAHASHI T., MAKISHIMA K., OHASHI T.
	Astrophys. J., Suppl. Ser., 133, 1-52 (2001)
	The ASCA medium sensitivity survey (the GIS catalog project): source catalog.
o	123 objects not correctly written, not in Simbad.
o	Table 2: <1AXG JHHMMSS+DDMM> N=1343.
Ref:	=2005ApJS..161..185U
by	UEDA Y. , ISHISAKI Y., TAKAHASHI T., MAKISHIMA K., OHASHI T.
	Astrophys. J., Suppl. Ser., 161, 185-223 (2005)
	The ASCA medium sensitivity survey (The GIS catalog project): source catalog II.
o	Table 2: <1AXG JHHMMSS+DDMM> N=1190.
=E=	Catalogue in electronic form as J/ApJS/133/1
=E=	Catalogue in electronic form as J/ApJS/161/185
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AXS
AXS	(ASCA satellite, X-ray Source)
*****	Avoid the usage of AXS, prefer AX
Origin	of the Acronym: L (1998ApJ...497L..29G)
Details on Acronym: [AY95]
[AY95]	(Alves+Yun, 1995) (Not yet in Simbad)
Write:	<<[AY95] A>>
N:	12
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Fig.2: 12 reddest objects in the Bok globule [CB88] 34.
in source:	[CB88] 34
Ref:	=1995ApJ...438L.107A
by	ALVES J.F. , YUN J.L.
	Astrophys. J., 438, 107-109 (1995)
	Multiple star formation in Bok globule CB 34.
o	Fig.2: <[AY95] A> (Nos A-G, L-N, P-Q)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AYM2020]
[AYM2020]	(Arellano Ferro+Yepez+Muneer S+, 2020)
Write:	<<[AYM2020] NGC 6254 VNN>>
N:	3
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	San Pedro Martir Observatory 0.84m telescope photometry of N=3 variable stars in the field of M10.
in source:	NGC 6254 = M 10
Ref:	=2020MNRAS.499.4026A
by	ARELLANO FERRO A. , YEPEZ M.A., MUNEER S., BUSTOS FIERRO I.H., SCHRODER K.P., GIRIDHAR S., CALDERON J.H.
	Mon. Not. R. Astron. Soc., 499, 4026-4039 (2020)
	The globular cluster M10: reassessment of stellar membership, distance, and age using its variable and HB stars.
o	Table 3: V1-V16 are <Cl* NGC 6254 SAW VNN>, V17-V34 are [RNS2018] NGC 6254 VNN in SIMBAD.
o	Table 3: <[AYM2020] NGC 6254 VNN> (Nos V35-V37).
=E=	Catalogue in electronic form as <J/MNRAS/499/4026/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Az
Az	(Azzopardi+)
*****	Avoid the usage of Az, prefer AzV
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [AZ2000]
[AZ2000]	(Alknis+Zharova, 2000) (Not yet in Simbad)
Write:	<<[AZ2000] NN>>
N:	18
Object:	* (SIMBAD class: Star)
Note:	Comparison stars of PT And. Fig.1: Finding chart.
Ref:	=2000IBVS.4909....1A
by	ALKSNIS A. , ZHAROVA A.V.
	IAU Inform. Bull. Var. Stars, 4909, 1-None (2000)
	PT Andromedae: the recent outburst and earlier ones.
o	Table 1: <[AZ2000] NN> (Nos 1-18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AZB2012]
[AZB2012]	(Anderson+Zavagno+Barlow+, 2012)
Write:	<<[AZB2012] GLLL.lll+BB.bbb>>
N:	126
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	N=126 HII regions. Use of data from the Herschel Hi-GAL survey, as well as WISE and the Spitzer MIPSGAL and GLIMPSE surveys.
Ref:	=2012A&A...537A...1A
by	ANDERSON L.D. , ZAVAGNO A., BARLOW M.J., GARCIA-LARIO P., NORIEGA-CRESPO A.
	Astron. Astrophys., 537A, 1-1 (2012)
	Distinguishing between HII regions and planetary nebulae with Hi-GAL, WISE, MIPSGAL, and GLIMPSE.
o	Table 1: <[AZB2012] GLLL.lll+BB.bbb> N=126.
=E=	Catalogue in electronic form as J/A+A/537/A1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AZB2016]
[AZB2016]	(Anastasopoulou+Zezas+Ballo+, 2016)
Write:	<<[AZB2016] NN>>
N:	26
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-S observations of N=26 X-ray sources in Arp 299.
in source:	APG 299
Ref:	=2016MNRAS.460.3570A
by	ANASTASOPOULOU K. , ZEZAS A., BALLO L., DELLA CECA R.
	Mon. Not. R. Astron. Soc., 460, 3570-3586 (2016)
	A deep Chandra observation of the interacting star-forming galaxy Arp 299.
o	Fig. 1, Table 1: <[AZB2016] NN> (Nos 1-26).
o	Warning: Name IC 694 used instead of NGC 3690A (IC 694 is another galaxy, cf the note in SIMBAD).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AZD2019]
[AZD2019]	(Antoniou+Zezas+Drake+, 2019)
Write:	<<[AZD2019] CXOU JHHMMSS.ss+DDMMSS.s>>
N:	123
Object:	HMXB (SIMBAD class: HighMassXBin = High Mass X-ray Binary)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of N=123 high-mass X-ray binaries (HMXBs) in the Small Magellanic Cloud.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2019ApJ...887...20A
by	ANTONIOU V. , ZEZAS A., DRAKE J.J., BADENES C., HABERL F., WRIGHT N.J., HONG J., DI STEFANO R., GAETZ T.J., LONG K.S., PLUCINSKY P.P., SASAKI M., WILLIAMS B.F., WINKLER P.F., (The SMC XVP Collaboration)
	Astrophys. J., 887, 20-20 (2019)
	Deep Chandra survey of the Small Magellanic Cloud. III. Formation efficiency of high-mass X-ray binaries.
o	Table 1: <[AZD2019] CXOU JHHMMSS.ss+DDMMSS.s> N=123.
=E=	Catalogue in electronic form as <J/ApJ/887/20/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [AZG2019]
[AZG2019]	(Anastasopoulou+Zezas+Gkiokas+, 2019) (Not yet in Simbad)
Write:	<<[AZG2019] NGC NNNN NN>>
N:	31+19
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS observations of N=31+19 discrete sources in the X-ray starburst galaxies NGC 3310 and NGC 2276.
in source:	NGC 3310
in source:	NGC 2276
Ref:	=2019MNRAS.483..711A
by	ANASTASOPOULOU K. , ZEZAS A., GKIOKAS V., KOVLAKAS K.
	Mon. Not. R. Astron. Soc., 483, 711-733 (2019)
	Do sub-galactic regions follow the galaxy-wide X-ray scaling relations? The example of NGC 3310 and NGC 2276.
o	Fig. 1, Table 1: <[AZG2019] NGC 3310 NN> (Nos 1-31). Fig. 2, Table 2: <[AZG2019] NGC 2276 NN> (Nos 1-19).
=E=	Catalogue in electronic form as <J/MNRAS/483/711/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AzGN
AzGN	(AzTEC/GOODS-N)
Write:	<<AzGN NN>>
N:	36
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	JCMT AzTEC 1.1mm survey of the GOODS-N field.
Ref:	=2008MNRAS.391.1227P
by	PERERA T.A. , CHAPIN E.L., AUSTERMANN J.E., SCOTT K.S., WILSON G.W., HALPERN M., POPE A., SCOTT D., YUN M.S., LOWENTHAL J.D., MORRISON G., ARETXAGA I., BOCK J.J., COPPIN K., CROWE M., FREY L., HUGHES D.H., KANG Y., KIM S., MAUSKOPF P.D.
	Mon. Not. R. Astron. Soc., 391, 1227-1238 (2008)
	An AzTEC 1.1mm survey of the GOODS-N field - I. Maps, catalogue and source statistics.
o	Table 1: <AzGN NN> (Nos 1-36).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AzLOCK
AzLOCK	(AzTEC Lockman Hole) (Not yet in Simbad)
*****	Avoid the usage of AzLOCK, prefer [ADP2010]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AzLOCK
AzLOCK	(AzTEC Lockman Hole)
*****	Avoid the usage of AzLOCK, prefer [MDI2012]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Azo
Azo	(Azzopardi+)
*****	Avoid the usage of Azo, prefer AzV
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [AZP2006]
[AZP2006]	(Azzaro+Zentner+Prada+, 2006)
Write:	<<[AZP2006] PGC NNNNNNN a>> <<[AZP2006] MCG +FF+FF-NNN a>> <<[AZP2006] NGC NNNN a>> <<[AZP2006] UGC NNNNN a>> <<[AZP2006] IC NNNN a>> <<[AZP2006] CGCG NN-NN a>>
N:	66
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Selected satellite galaxies (N=66) about galaxy primaries (N=43) extracted from the SDSS.
Ref:	=2006ApJ...645..228A
by	AZZARO M. , ZENTNER A.R., PRADA F., KLYPIN A.A.
	Astrophys. J., 645, 228-239 (2006)
	The peculiar velocities of satellites of external disk galaxies.
o	Table 3: <[AZP2006] PGC NNNNNNN a>, <[AZP2006] MCG +FF+FF-NNN a>, <[AZP2006] NGC NNNN a>, <[AZP2006] UGC NNNNN a>, <[AZP2006] IC NNNN a>, <[AZP2006] CGCG NN-NN a>, N=66.
=E=	Catalogue in electronic form as J/ApJ/645/228
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: AzSXDF
AzSXDF	(AzTEC SXDF) (Not yet in Simbad)
*****	Avoid the usage of AzSXDF, prefer [ADP2010]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AzTEC
AzTEC	(AzTEC) (Not yet in Simbad)
*****	Avoid the usage of AzTEC, prefer [AWA2011]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AzTEC
AzTEC	(AzTEC camera)
Write:	<<AzTEC NN>> <<AzTEC NN.W>> <<AzTEC JHHMMSS.ss+DDMMSS.s>>
N:	34+52+49+114+198+125
Object:	G + (smm) (SIMBAD class: Galaxy)
Note:	1.1mm observations with the AzTEC camera mounted on the James Clerk Maxwell Telescope (JCMT) or the Atacama Submillimeter Telescope Experiment (ASTE).
in source:	NAME COSMOS Field
in source:	NAME GOODS South Field
in source:	NAME Lockman Hole
in source:	NAME SXDF
in source:	SSA 22
Ref:	=2007ApJ...671.1531Y
by	YOUNGER J.D. , FAZIO G.G., HUANG J.-S., YUN M.S., WILSON G.W., ASHBY M.L.N., GURWELL M.A., LAI K., PECK A.B., PETITPAS G.R., WILNER D.J., IONO D., KOHNO K., KAWABE R., HUGHES D.H., ARETXAGA I., WEBB T., MARTINEZ-SANSIGRE A., KIM S., SCOTT K.S., AUSTERMANN J., PERERA T., LOWENTHAL J.D., SCHINNERER E., SMOLCIC V.
	Astrophys. J., 671, 1531-1537 (2007)
	Evidence for a population of high-redshift submillimeter galaxies from interferometric imaging.
o	Table 1: <AzTEC N> (Nos 1-7).
Ref:	=2008MNRAS.385.2225S
by	SCOTT K.S. , AUSTERMANN J.E., PERERA T.A., WILSON G.W., ARETXAGA I., BOCK J.J., HUGHES D.H., KANG Y., KIM S., MAUSKOPF P.D., SANDERS D.B., SCOVILLE N., YUN M.S.
	Mon. Not. R. Astron. Soc., 385, 2225-2238 (2008)
	AzTEC millimetre survey of the COSMOS field - I. Data reduction and source catalogue.
o	Table 1: <AzTEC JHHMMSS.ss+DDMMSS.s> N=52.
Ref:	=2009ApJ...704..803Y
by	YOUNGER J.D. , FAZIO G.G., HUANG J.-S., YUN M.S., WILSON G.W., ASHBY M.L.N., GURWELL M.A., PECK A.B., PETITPAS G.R., WILNER D.J., HUGHES D.H., ARETXAGA I., KIM S., SCOTT K.S., AUSTERMANN J., PERERA T., LOWENTHAL J.D.
	Astrophys. J., 704, 803-812 (2009)
	The AzTEC/SMA interferometric imaging survey of submillimeter-selected high-redshift galaxies.
o	Table 1: <AzTEC NN.W> (Nos 8-15, 11.N, 11.S, 14.E, 14.W) added = <AzTEC JHHMMSS.ss+DDMMSS.s> N=11.
Ref:	=2010MNRAS.401..160A
by	AUSTERMANN J.E. , DUNLOP J.S., PERERA T.A., SCOTT K.S., WILSON G.W., ARETXAGA I., HUGHES D.H., ALMAINI O., CHAPIN E.L., CHAPMAN S.C., CIRASUOLO M., CLEMENTS D.L., COPPIN K.E.K., DUNNE L., DYE S., EALES S.A., EGAMI E., FARRAH D., FERRUSCA D., FLYNN S., HAIG D., HALPERN M., IBAR E., IVISON R.J., VAN KAMPEN E., KANG Y., KIM S., LACEY C., LOWENTHAL J.D., MAUSKOPF P.D., McLURE R.J., MORTIER A.M.J., NEGRELLO M., OLIVER S., PEACOCK J.A., POPE A., RAWLINGS S., RIEKE G., ROSEBOOM I., ROWAN-ROBINSON M., SCOTT D., SERJEANT S., SMAIL I., SWINBANK A.M., STEVENS J.A., VELAZQUEZ M., WAGG J., YUN M.S.
	Mon. Not. R. Astron. Soc., 401, 160-176 (2010)
	AzTEC half square ° survey of the SHADES fields - I. Maps, catalogues and source counts.
o	Tables 1-2, col(1): <AzTEC JHHMMSS.ss+DDMMSS.s> N=86 = Tables 1-2, col(2): <[ADP2010] AzLOCK.NN> (Nos 1-86). Table 3, col(1): <AzTEC JHHMMSS.ss+DDMMSS.s> N=28 = Table 3, col(2): <[ADP2010] AzSXDF.NN> (Nos 1-28).
Ref:	=2010MNRAS.405.2260S
by	SCOTT K.S. , YUN M.S., WILSON G.W., AUSTERMANN J.E., AGUILAR E., ARETXAGA I., EZAWA H., FERRUSCA D., HATSUKADE B., HUGHES D.H., IONO D., GIAVALISCO M., KAWABE R., KOHNO K., MAUSKOPF P.D., OSHIMA T., PERERA T.A., RAND J., TAMURA Y., TOSAKI T., VELAZQUEZ M., WILLIAMS C.C., ZEBALLOS M.
	Mon. Not. R. Astron. Soc., 405, 2260-2278 (2010)
	Deep 1.1mm-wavelength imaging of the GOODS-S field by AzTEC/ASTE - I. Source catalogue and number counts.
o	Table 1, col(1): <[SYW2010] AzTEC/GSNN.N> (Nos 1-2, 2.1-2.2, 3-47) = Table 1, col(2): <AzTEC JHHMMSS.ss+DDMMSS.s> N=49.
Ref:	=2011MNRAS.411..102H
by	HATSUKADE B. , KOHNO K., ARETXAGA I., AUSTERMANN J.E., EZAWA H., HUGHES D.H., IKARASHI S., IONO D., KAWABE R., KHAN S., MATSUO H., MATSUURA S., NAKANISHI K., OSHIMA T., PERERA T., SCOTT K.S., SHIRAHATA M., TAKEUCHI T.T., TAMURA Y., TANAKA K., TOSAKI T., WILSON G.W., YUN M.S.
	Mon. Not. R. Astron. Soc., 411, 102-116 (2011)
	AzTEC/ASTE 1.1-mm survey of the AKARI Deep Field South: source catalogue and number counts.
o	Table 2, col(1): <AzTEC JHHMMSS.ss+DDMMSS.s> N=198.
Ref:	=2014MNRAS.440.3462U
by	UMEHATA H. , TAMURA Y., KOHNO K., HATSUKADE B., SCOTT K.S., KUBO M., YAMADA T., IVISON R.J., CYBULSKI R., ARETXAGA I., AUSTERMANN J., HUGHES D.H., EZAWA H., HAYASHINO T., IKARASHI S., IONO D., KAWABE R., MATSUDA Y., MATSUO H., NAKANISHI K., OSHIMA T., PERERA T., TAKATA T., WILSON G.W., YUN M.S.
	Mon. Not. R. Astron. Soc., 440, 3462-3478 (2014)
	AzTEC/ASTE 1.1-mm survey of SSA22: Counterpart identification and photometric redshift survey of submillimetre galaxies.
o	Table 2, col(1): <AzTEC JHHMMSS.ss+DDMMSS.s> N=125 = Table 2, col(2): <[UTK2014] SSA22-AzTECNNN> (Nos 1-125). Table 3: <[UTK2014] SSA22-AzTEC-SupNN> (Nos 1-17). Table 5: <[UTK2014] SSA22-AzNNNa> N=83 among (Nos Az1a-Az117a), <[UTK2014] JHHMMSS.ss+DDMMSS.s> N=21+76.
Ref:	=2015A&A...577A..29M
by	MIETTINEN O. , SMOLCIC V., NOVAK M., ARAVENA M., KARIM A., MASTERS D., RIECHERS D.A., BUSSMANN R.S., McCRACKEN H.J., ILBERT O., BERTOLDI F., CAPAK P., FERUGLIO C., HALLIDAY C., KARTALTEPE J.S., NAVARRETE F., SALVATO M., SANDERS D., SCHINNERER E., SHETH K.
	Astron. Astrophys., 577A, 29-29 (2015)
	(Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies. I. Multiwavelength identifications and redshift distribution.
o	Fig. 1, Tables 1-2: <AzTEC NN> (Nos 16-30). Fig. 1, Table 3: <[MSN2015] AzTEC NNa> N=14 among (Nos AzTEC 17a and AzTEC 29a-b).
=E=	Catalogue in electronic form as J/MNRAS/385/2225
=E=	Catalogue in electronic form as <J/MNRAS/405/2260/>
=E=	Catalogue in electronic form as J/MNRAS/411/102
=E=	Catalogue in electronic form as <J/MNRAS/401/160/>
=E=	Catalogue in electronic form as <J/MNRAS/440/3462/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AzTEC/C
AzTEC/C	(AzTEC/COSMOS) (Not yet in Simbad)
*****	Avoid the usage of AzTEC/C, prefer [AWA2011]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AzTEC/COSMOS
AzTEC/COSMOS	(AzTEC COSMOS)
*****	Avoid the usage of AzTEC/COSMOS, prefer [DWS2012]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AzTEC/GN
AzTEC/GN	(AzTEC GOODS North)
*****	Avoid the usage of AzTEC/GN, prefer [DWS2012]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AzTEC/GS
AzTEC/GS	(AzTEC GOODS South)
*****	Avoid the usage of AzTEC/GS, prefer [DWS2012]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AzTEC/LH
AzTEC/LH	(AzTEC Lockman Hole)
*****	Avoid the usage of AzTEC/LH, prefer [DWS2012]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AzTEC/SXDF
AzTEC/SXDF	(AzTEC SXDF)
*****	Avoid the usage of AzTEC/SXDF, prefer [DWS2012]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AzUDS
AzUDS	(AzTEC SXDF/UDS)
*****	Avoid the usage of AzUDS, prefer [MDI2012]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: AzV
AzV	(Azzopardi+Vigneau+)= AV = (Az) = (Azo) = AzVi
Write:	<<AzV NNNa>> <<AzV NNNF>>
N:	524+124
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-506) alf = 0h41 - 1h22 (1975) Format 'NNNa': the letter in the format means inclusion between two consecutive stars of the previous lists ordered in RA. Format 'NNNF' stands for Foreground stars, (Nos 1F-124F) Finding Charts
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1975A&AS...22..285A
by	AZZOPARDI M. , VIGNEAU J., MACQUET M.
	Astron. Astrophys., Suppl. Ser., 22, 285-321 (1975)
	List of 506 stars probable Small Magellanic Cloud members.
o	Catalogue: <AzV NNN> (Nos 1-506)
Ref:	=1979A&AS...35..353A
by	AZZOPARDI M. , VIGNEAU J.
	Astron. Astrophys., Suppl. Ser., 35, 353-369 (1979)
	Small Magellanic Cloud, additional list of probable members and foreground stars.
o	Table 1: <AzV NNNa> N=18 among (Nos 1a-502a). Table 2: <AzV NNNF> (Nos 1F-124F).
Ref:	=1982A&AS...50..291A
by	AZZOPARDI M. , VIGNEAU J.
	Astron. Astrophys., Suppl. Ser., 50, 291-376 (1982)
	Catalogue of the Small Magellanic Cloud star members.
o	Table II: <AzV NNNA> (Nos 1-506) N=524
=E=	Catalogue in electronic form as V/13
Origin	of the Acronym: L = Found in the literature
Details on Acronym: AzVi
AzVi	(Azzopardi+Vigneau+)
====>	Equivalent to: AzV
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [AZW2014]
[AZW2014]	(An+Zheng+Wang+, 2014)
Write:	<<[AZW2014] NN>>
N:	56
Object:	Halpha emitter (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	CFHT WIRCam observations of N=56 Hα emission-line galaxies (ELGs) at z=2.24, in the Extended Chandra Deep Field South.
in source:	NAME ECDFS
Ref:	=2014ApJ...784..152A
by	AN F.X. , ZHENG X.Z., WANG W.-H., HUANG J.-S., KONG X., WANG J.-X., FANG G.W., ZHU F., GU Q.-S., WU H., HAO L., XIA X.-Y.
	Astrophys. J., 784, 152 (2014)
	The properties of Hα emission-line galaxies at z = 2.24.
o	Tables 1-2: <[AZW2014] NN> (Nos 1-56).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: B
B	(Blue stellar obj.)
*****	Avoid the usage of B, prefer [A81b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: B
B	(Braccesi, 1968)
*****	Avoid the usage of B, prefer [B68b]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: B
B	(Blecha)
*****	Avoid the usage of B, prefer [B86c]
Origin	of the Acronym: L (2000MNRAS.311..673B)
Details on Acronym: B
B	(Baade)
*****	Avoid the usage of B, prefer BA
Origin	of the Acronym: L = Found in the literature
Details on Acronym: B
B	(Barnard)
*****	Avoid the usage of B, prefer Barnard
Origin	of the Acronym: L = Found in the literature
Details on Acronym: B
B	(Boulesteix+)
*****	Avoid the usage of B, prefer BCLMP
Origin	of the Acronym: L (1980A&AS...40...67D,1996ApJ...466..750L)
Details on Acronym: B
B	(Bothun+)
*****	Avoid the usage of B, prefer [BCS89]
Origin	of the Acronym: L (1997A&AS..124....1J)
Details on Acronym: B
B	(Blitz+)
*****	Avoid the usage of B, prefer BFS
Origin	of the Acronym: L = Found in the literature
Details on Acronym: B
B	(Bailey+)
*****	Avoid the usage of B, prefer BHA
Origin	of the Acronym: L (1989ApJ...336..752R)
Details on Acronym: B
B	(Barsony+)
*****	Avoid the usage of B, prefer BKLT
Origin	of the Acronym: L (2001A&A...372..173B)
Details on Acronym: B
B	(Butcher+)
*****	Avoid the usage of B, prefer [BO85]
Origin	of the Acronym: L (2000MNRAS.313..469S)
Details on Acronym: B
B	(Bologna obs.)
*****	Avoid the usage of B, prefer Bol
Origin	of the Acronym: L (2007AJ....133.2764B)
Details on Acronym: B
B	(Bedin+)
Origin	of the Acronym: L (2007AJ....134.2168P)
Details on Acronym: B
B	(Bruck)
*****	Avoid the usage of B, prefer Bruck
Origin	of the Acronym: L (1998AcA....48..175P)
Details on Acronym: B
B	(Belloni+)
*****	Avoid the usage of B, prefer BVS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: B
B	(Baud+)
*****	Avoid the usage of B, prefer BYB
Origin	of the Acronym: L (1998A&A...338..977C)
Details on Acronym: B
B	(Boss)
*****	Avoid the usage of B, prefer GC
Details on Acronym: B
B	(Cloud Complex labelled B)
Note:	HVC cloud B
*****	Avoid the usage of B, prefer [H68]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: B
B	(Byurakan)
*****	Avoid the usage of B, prefer [H83b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: B
B	(Brundage)
*****	Avoid the usage of B, prefer SB
Details on Acronym: B
B	(Batten)
*****	Avoid the usage of B, prefer SBC7
Details on Acronym: B
B	(Baade)
*****	Avoid the usage of B, prefer [SN45]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: B
B	(Blue)
*****	Avoid the usage of B, prefer [TB95]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: B
B	(Baade)
*****	Avoid the usage of B, prefer [V62]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: B		B
B	B	(Bahcall+Bahcall)
*****	Avoid the usage of B	B, prefer [BB70]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: B-HiZELS
B-HiZELS	(Bootes-HiZELS)
Write:	<<B-HiZELS NN>> <<B-HiZELS NB392 NN>> <<B-HiZELS stV NN>> <<B-HiZELS NB501 NN>> <<B-HiZELS NB921 NNNN>> <<B-HiZELS NBH NNN>> <<B-HiZELS NBK NNN>>
N:	42+57+39+65+1161+301+255
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	INT WFC (NB392, NB501, stV), Subaru SuprimeCam (NB921), UKIRT WFCAM (NB_H, NB_K) observations of N=42+57+39+65+1161+301+255 emission-line galaxies, as part of High-z Emission-Line Survey in the Bootes field.
in source:	NAME Bootes Field
Ref:	=2017MNRAS.471..629M
by	MATTHEE J. , SOBRAL D., BEST P., SMAIL I., BIAN F., DARVISH B., ROTTGERING H., FAN X.
	Mon. Not. R. Astron. Soc., 471, 629-649 (2017)
	Bootes-HiZELS: an optical to near-infrared survey of emission-line galaxies at z = 0.4-4.7.
o	Table C1: <B-HiZELS NN> (Nos 1-42). Table D1: <B-HiZELS NB392 NN> (Nos 1-57). Table D2: <B-HiZELS stV NN> (Nos 1-39). Table D3: <B-HiZELS NB501 NN> (Nos 1-65). Table D4: <B-HiZELS NB921 NNNN> (Nos 1-1161). Table D5: <B-HiZELS NBH NNN> (Nos 1-301). Table D6: <B-HiZELS NBK NNN> (Nos 1-255).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: B-OB
B-OB	(Battinelli, OB assoc.)
*****	Avoid the usage of B-OB, prefer [B91]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: 1B
1B	(1st BATSE catalog)= BATSE = (GRB)
Write:	<<1B YYMMDDA>>
N:	260
Object:	(Gamma) (SIMBAD class: gammaBurst = Gamma-ray Burst)
Stat:	is completely incorporated in Simbad
Note:	BATSE experiment on the CGRO satellite, N=260 cosmic gamma-ray bursts during the period 1991 April 19 to 1992 March 5. see also 2B, 3B, 4B
Ref:	=1994ApJS...92..229F
by	FISHMAN G.J. , MEEGAN C.A., WILSON R.B., BROCK M.N., HORACK J.M., KOUVELIOTOU C., HOWARD S., PACIESAS W.S., BRIGGS M.S., PENDLETON N., KOSHUT T.M., MALLOZZI R.S., STOLLBERG M., LESTRADE J.P.
	Astrophys. J., Suppl. Ser., 92, 229-283 (1994)
	The first BATSE Gamma-ray burst catalog.
o	Table 1, col (1): <Trigger NNNN> N=260, Table 1, col (2): <1B YYMMDDA> N=260
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: B1
B1	(1st Bologna survey)= B1S
Write:	<<B1 HHMM+DD>>
N:	654+38
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Table I: N=654. Table II: N=38 supplementary sources.
Ref:	=1965NCimB..40....1B
by	BRACCESI A. , CECCARELLI M., FANTI R., GELATO G., GIOVANNINI C., HARRIS D., ROSATELLI C., SINIGAGLIA G., VOLDERS L.
	Nuovo Cimento B, 40, 1-33 (1965)
	A catalogue of radiosources from declination -30° to -20° at 408 MHz.
o	Tables I, II: <B1 HHMM+DDA> N=654+38.
Details on Acronym: B1
B1	(Bolton, list 1)
*****	Avoid the usage of B1, prefer BWSS
Details on Acronym: [B10]
[B10]	(Boss, 1910)= (Boss) = (PGC)
Write:	<<[B10] NNNN>>
N:	6188
Object:	* (SIMBAD class: Star)
Note:	Preliminary General Catalogue of 6188 stars (Nos 1-6188) for the Epoch 1900. Superseded by GC catalogue Published in Carnegie Publ. 115.
Auth.:	BOSS L.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: B1S
B1S	(1st Bologna survey, Suppl.)
*****	Avoid the usage of B1S, prefer B1
Details on Acronym: 2B
2B	(2nd BATSE catalog)= BATSE = (GRB)
Write:	<<2B YYMMDDA>>
N:	585
Object:	(Gamma) (SIMBAD class: gammaBurst = Gamma-ray Burst)
Stat:	is completely incorporated in Simbad
Note:	BATSE experiment on the CGRO satellite, N=585 cosmic gamma-ray bursts during the period 1991 April 19 to 1993 March 9. see also 1B, 3B, 4B
Auth.:	MEEGAN C.A.+
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: B2
B2	(2nd Bologna Survey)= (B2.1) = (B2.2) = (B2.3) = (B2.4)
Write:	<<B2 HHMM+DDA>>
N:	3235+3013+3227+448
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	In the 4 parts of the second Bologna catalogue (4 references) the full name always starts by B2, followed by truncated 1950 position, eventually followed by a letter A,B,C... In the electronic catalog, the authors have introduced a new designation B2.1, B2.2, B2.3 and B2.4 for the part number 1 to 4 of the full catalogue, to have unique names.
Ref:	=1970A&AS....1..281C
by	COLLA G. , FANTI C., FANTI R., FICARRA A., FORMIGGINI L., GANDOLFI E., GRUEFF G., LARI C., PADRIELLI L., ROFFI G., TOMASI P., VIGOTTI M.
	Astron. Astrophys., Suppl. Ser., 1, 281-317 (1970)
	A catalogue of 3235 radio sources at 408 MHz.
o	Catalogue: <B2 HHMM+DDA> = <B2.1 HHMM+DDA> N=3235.
Ref:	=1972A&AS....7....1C
by	COLLA G. , FANTI C., FANTI R., FICARRA A., FORMIGGINI L., GANDOLFI E., LARI C., MARANO B., PADRIELLI L., TOMASI P.
	Astron. Astrophys., Suppl. Ser., 7, 1-34 (1972)
	The B2 catalogue of radio sources - second part.
o	Catalogue: <B2 HHMM+DDA> = <B2.2 HHMM+DDA> N=3013.
Ref:	=1973A&AS...11..291C
by	COLLA G. , FANTI C., FANTI R., FICARRA A., FORMIGGINI L., GANDOLFI E., GIOIA I., LARI C., MARANO B., PADRIELLI L., TOMASI P.
	Astron. Astrophys., Suppl. Ser., 11, 291-325 (1973)
	The B2 catalogue of radio sources - third part.
o	Catalogue: <B2 HHMM+DDA> = <B2.3 HHMM+DDA> N=3227.
Ref:	=1974A&AS...18..147F
by	FANTI C. , FANTI R., FICARRA A., PADRIELLI L.
	Astron. Astrophys., Suppl. Ser., 18, 147-156 (1974)
	The B2 catalogue of radio sources - fourth part.
o	Catalogue: <B2 HHMM+DDA> = <B2.4 HHMM+DDA> N=448.
=E=	Catalogue in electronic form as VIII/36
Details on Acronym: B2
B2	(Bolton, list 2)
*****	Avoid the usage of B2, prefer BSS
Details on Acronym: B2.1
B2.1	(2nd Bologna Survey, Part 1)
Note:	See also B2
*****	Avoid the usage of B2.1, prefer B2
Details on Acronym: B2.2
B2.2	(2nd Bologna Survey, Part 2)
Note:	See also B2
*****	Avoid the usage of B2.2, prefer B2
Details on Acronym: B2.3
B2.3	(2nd Bologna Survey, Part 3)
Note:	See also B2
*****	Avoid the usage of B2.3, prefer B2
Details on Acronym: B2.4
B2.4	(2nd Bologna Survey, Part 4)
Note:	See also B2
*****	Avoid the usage of B2.4, prefer B2
Details on Acronym: [B2001]
[B2001]	(Bottini, 2001)= ([B2001a])
Write:	<<[B2001] ACO NNNN A>> <<[B2001] MS HHMM+DDMM A>>
N:	265
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	N=265 Galaxies in 52 ClG.
Ref:	=2001AJ....121.1294B
by	BOTTINI D.
	Astron. J., 121, 1294-1305 (2001)
	A kinematic search for bound populations around brightest cluster members in a sample of 52 clusters of galaxies.
o	Table 2: <[B2001] ACO NNNN A>, <[B2001] MS HHMM+DDMM A>, N=265.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2001a]
[B2001a]	(Bottini, 2001)
*****	Avoid the usage of [B2001a], prefer [B2001]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2001b]
[B2001b]	(Bourke, 2001)= (IRS)
Write:	<<[B2001b] IRS N>>
N:	2
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	ISO observations. Protostellar sources in BHR 71. See also [GMC2004]
in source:	BHR 71
Ref:	=2001ApJ...554L..91B
by	BOURKE T.L.
	Astrophys. J., 554, 91-94 (2001)
	IRAS 11590-6452 in BHR 71: a binary protostellar system.
o	Fig.1, Table 1: <[B2001b] IRS N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2001c]
[B2001c]	(Bukhmastova, 2001) (Not yet in Simbad)
Write:	<<[B2001c] NNNN>>
N:	8382
Object:	QSO-G pair (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	New catalog of 8382 close quasar-galaxy pairs. It could have several galaxies near a single quasar, and several quasars near a single galaxy (11358 objects).
Ref:	=2001ARep...45..581B
by	BUKHMASTOVA Y.L.
	Astron. Rep., 45, 581-590 (2001)
	Properties of quasar-galaxy associations and gravitational mesolensing by halo objects.
o	2001AZh....78..675B
o	Catalog: <[B2001c] NNNN>(Nos 1-8382).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2002]
[B2002]	(Burton, 2002)= [B2002a] (Not yet in Simbad)
Write:	<<[B2002] N>>
N:	4
Object:	Region (SIMBAD class: Region = Region defined in the Sky)
Note:	N=4 regions of molecular H2 emission in M 8. Coordinates are position of peak emission.
in source:	M 8 = Lagoon Nebula
Ref:	=2002PASA...19..260B
by	BURTON M.G.
	Publications - Astron. Soc. Australia, 19, 260-264 (2002)
	Molecular hydrogen in the Lagoon : H2 line emission from Messier 8.
o	Table 1: <[B2002] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2002a]
[B2002a]	(Burton, 2002) (Not yet in Simbad)
*****	Avoid the usage of [B2002a], prefer [B2002]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2002b]
[B2002b]	(Best, 2002)
Write:	<<[B2002b] HzClHHMM-850.N>> <<[B2002b] HzClHHMMa-850.N>> <<[B2002b] HzClHHMMa-450.N>>
N:	17
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SCUBA observations of smm sources in four clusters of galaxies, at 850mu.m and 450mu.m. In the format 'HHMM' are J2000 coordinates of the R.A. of each cluster.
in source:	ClG J0023+0423
in source:	ClG J0848+4453
in source:	ClG J1604+4304
in source:	ClG J1604+4321
Ref:	=2002MNRAS.336.1293B
by	BEST P.N.
	Mon. Not. R. Astron. Soc., 336, 1293-1303 (2002)
	An excess of submillimetre sources towards z ~ 1 clusters.
o	Table 2: <[B2002b] HzClHHMM-850.N>, <[B2002b] HzClHHMMa-850.N>, <[B2002b] HzClHHMMa-450.N>, N=17.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2002c]
[B2002c]	(Boschin, 2002)
Write:	<<[B2002c] NN>>
N:	36
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	First results of a search for clusters of galaxies in Chandra ACIS pointed observations at high latitude.
Ref:	=2002A&A...396..397B
by	BOSCHIN W.
	Astron. Astrophys., 396, 397-409 (2002)
	A deep cluster survey in Chandra archival data. First results.
o	Table 1: <[B2002c] NN> (Nos 1-36).
=E=	Catalogue in electronic form as J/A+A/396/397
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2003]
[B2003]	(Basilakos, 2003)
Write:	<<[B2003] NN>>
N:	57
Object:	Supercluster of G (SIMBAD class: SuperClG = Supercluster of Galaxies)
Note:	Search for superclusters in the SDSS CE cluster catalogue (2002AJ....123.1807G) using an approach based on differential geometry.
Ref:	=2003MNRAS.344..602B
by	BASILAKOS S.
	Mon. Not. R. Astron. Soc., 344, 602-606 (2003)
	Shape statistics of Sloan Digital Sky Survey superclusters.
o	Table 1: <[B2003] NN> (Nos 1-57).
=E=	Catalogue in electronic form as J/MNRAS/344/602
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2004]
[B2004]	(Boles, 2004)= ([B2004a])
Write:	<<[B2004] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of SN 2004DF.
Ref:	=2004IAUC.8374....1B
by	BOLES T.
	IAU Circ., 8374, 1-None (2004)
	Supernova 2004df.
o	<[B2004] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2004a]
[B2004a]	(Boles, 2004)
*****	Avoid the usage of [B2004a], prefer [B2004]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2004b]
[B2004b]	(Barris, 2004)= (SN)
Write:	<<[B2004b] fFFFFa>>
N:	70
Object:	Poss. SN (SIMBAD class: Supernova_Candidate = SuperNova Candidate)
Note:	Subaru Suprime-Cam and CFHT 12K camera observations of possible supernovae in selected fields, within the IfA Deep Survey.
Ref:	=2004PhDT.........8B
by	BARRIS B.J.
	PhDT, , 8 (2004)
	Type Ia supernovae at high redshift.
o	Table 4.6: <[B2004b] fFFFFa> N=70.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2005]
[B2005]	(Boles, 2005)= ([B2005a])
Write:	<<[B2005] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Apparent host galaxy of SN 2005C.
Ref:	=2005IAUC.8463....2B
by	BOLES T.
	IAU Circ., 8463, 2-None (2005)
	Supernova 2005C.
o	<[B2005] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2005a]
[B2005a]	(Boles, 2005)
*****	Avoid the usage of [B2005a], prefer [B2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2005b]
[B2005b]	(Bloom, 2005)
Write:	<<[B2005b] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	The red source is identified as the host galaxy of GRB 051221 in 2005GCN..4375....1S.
Ref:	=2005GCN..4367....1B
by	BLOOM J.S.
	GRB Coordinates Network, Circular Service, 4367, 1-None (2005)
	GRB051221: K-band source.
o	<[B2005b] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2006]
[B2006]	(Berger, 2006)
Write:	<<[B2006] JHHMMSS.s+DDMMSS>>
N:	87
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 8.5GHz observations of 90 dwarf stars and brown dwarfs of spectral type M5-T8.
Ref:	=2006ApJ...648..629B
by	BERGER E.
	Astrophys. J., 648, 629-636 (2006)
	Radio observations of a large sample of late M, L, and T dwarfs: the distribution of magnetic field strengths.
o	Table 1: <[B2006] JHHMMSS.s+DDMMSS> N=87.
=E=	Catalogue in electronic form as J/ApJ/648/629
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2007]
[B2007]	(Bonanos, 2007)= ([B2007a])
Write:	<<[B2007] JHHMMSS.ss+DDMMSS.s>>
N:	129
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Photometry of Cl Westerlund 1 at the 1m Swope telescope at Las Campanas Observatory.
in source:	Cl Westerlund 1
Ref:	=2007AJ....133.2696B
by	BONANOS A.Z.
	Astron. J., 133, 2696-2708 (2007)
	Variability of young massive stars in the galactic super star cluster Westerlund 1.
o	Table 2: <[B2007] JHHMMSS.ss+DDMMSS.s> N=129.
=E=	Catalogue in electronic form as J/AJ/133/2696
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2007a]
[B2007a]	(Bonanos, 2007)
*****	Avoid the usage of [B2007a], prefer [B2007]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2007b]
[B2007b]	(Beck, 2007)
Write:	<<[B2007b] source A>> <<[B2007b] JHHMMSS.s+DDMMSS>>
N:	2+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA radio continuum observations of NGC 6946: a close pair of bright background sources is observed, and another background pair.
Ref:	=2007A&A...470..539B
by	BECK R.
	Astron. Astrophys., 470, 539-556 (2007)
	Magnetism in the spiral galaxy NGC 6946: magnetic arms, depolarization rings, dynamo modes, and helical fields.
o	Text, paragr.3.7: <[B2007b] source A> (Nos A-B), <[B2007b] JHHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2007c]
[B2007c]	(Berger, 2007)
Write:	<<[B2007c] JHHMMSS.sss+DDMMSS.ss>>
N:	9
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Magellan Clay 6.5m telescope LDSS3 spectroscopic observations of the cluster ACO S 995. See also [BNB2006].
in source:	ACO S 995
Ref:	=2007GCN..5995....1B
by	BERGER E.
	GCN, 5995, 1 (2007)
	GRB 061201: nearby galaxy cluster Abell 995 is at z=0.0865.
o	ACO 995 is a misprint for ACO S 995.
o	<[B2007c] JHHMMSS.sss+DDMMSS.ss> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2008]
[B2008]	(Brentjens, 2008)= ([B2008a])
Write:	<<[B2008] NN>>
N:	11
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Deep polarimetric Westerbork observations of discrete sources in ACO 2256.
in source:	ACO 2256
Ref:	=2008A&A...489...69B
by	BRENTJENS M.A.
	Astron. Astrophys., 489, 69-83 (2008)
	Deep Westerbork observations of Abell 2256 at 350 MHz.
o	Fig.11, Table 3: <[B2008] NN> (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2008a]
[B2008a]	(Brentjens, 2008)
*****	Avoid the usage of [B2008a], prefer [B2008]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2008b]
[B2008b]	(Bhattacharyya, 2008)
Write:	<<[B2008b] Source A>>
N:	1
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Possible infrared and optical counterpart of CXOU J172337.5-374442. N=1 point-like optical and IR source at 0.15 arcsec.
Ref:	=2008MNRAS.391L.117B
by	BHATTACHARYYA S.
	Mon. Not. R. Astron. Soc., 391L, 117-121 (2008)
	A new interesting source in Chandra field: a pulsar wind nebula?
o	Text: <[B2008b] Source A> (No. A).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2009]
[B2009]	(Berger, 2009)= ([B2009a])
Write:	<<[B2009] JHHMMSS.ss+DDMMSS.ss>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Note:	N=2 SDSS candidate host galaxies for GRB 090313.
Ref:	=2009GCN..8984....1B
by	BERGER E.
	GCN, 8984, 1 (2009)
	GRB 090313: SDSS object underlying the optical afterglow position.
o	<[B2009] JHHMMSS.ss+DDMMSS.ss> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2009a]
[B2009a]	(Berger, 2009)
*****	Avoid the usage of [B2009a], prefer [B2009]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2009b]
[B2009b]	(Boles, 2009)
Write:	<<[B2009b] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	Poss. SN (SIMBAD class: Supernova_Candidate = SuperNova Candidate)
Stat:	is completely incorporated in Simbad
Note:	Possible SN in UGC 2773.
Ref:	=2009CBET.1931....1B
by	BOLES T.
	CBET, 1931, 1 (2009)
	Possible supernova in UGC 2773.
o	<[B2009b] J033207.24+474739.6> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2010]
[B2010]	(Bohlin, 2010)= ([B2010a])
Write:	<<[B2010] C26202>> <<[B2010] SF1615+001A>> <<[B2010] SNAP-2>>
N:	3
Object:	* (SIMBAD class: Star)
Note:	HST spectrophotometry for solar analogs.
Ref:	=2010AJ....139.1515B
by	BOHLIN R.C.
	Astron. J., 139, 1515-1520 (2010)
	Hubble space telescope spectrophotometry and models for solar analogs.
o	Table 2: Stars PNNN-A are GSPC P NNN-A in Simbad.
o	Table 2: <[B2010] C26202>, <[B2010] SF1615+001A>, <[B2010] SNAP-2>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2010a]
[B2010a]	(Bohlin, 2010) (Not yet in Simbad)
*****	Avoid the usage of [B2010a], prefer [B2010]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2010b]
[B2010b]	(Barnard, 2010)
Write:	<<[B2010b] NGC253 ULXN>>
N:	3
Object:	ULX (SIMBAD class: ULX = Ultra-luminous X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observation of the nearby spiral galaxy NGC 253 yielded N=3 ultraluminous X-ray sources.
in source:	NGC 253
Ref:	=2010MNRAS.404...42B
by	BARNARD R.
	Mon. Not. R. Astron. Soc., 404, 42-47 (2010)
	In-depth studies of the NGC253 ULXs with XMM-Newton: remarkable variability in ULX1, and evidence for extended coronae.
o	ULXs 1, 2, 3 in NGC 253 are respectively [BGK2008] S64, S102, S123 in SIMBAD.
o	Table 1: <[B2010b] NGC253 ULXN> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2011]
[B2011]	(Bresolin, 2011)= ([B2011a])
Write:	<<[B2011] NN>>
N:	36
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Gemini North GMOS observations of NGC 4258.
in source:	NGC 4258
Ref:	=2011ApJ...729...56B
by	BRESOLIN F.
	Astrophys. J., 729, 56 (2011)
	Revisiting the abundance gradient in the maser host galaxy NGC 4258.
o	Fig. 1, Table 2: <[B2011] NN> (Nos 1-36).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2011a]
[B2011a]	(Bresolin, 2011)
*****	Avoid the usage of [B2011a], prefer [B2011]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2011b]
[B2011b]	(Bresolin, 2011)
Write:	<<[B2011b] NN>>
N:	25
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Gemini North GMOS observations of M 33.
in source:	M 33 = NGC 598
Ref:	=2011ApJ...730..129B
by	BRESOLIN F.
	Astrophys. J., 730, 129 (2011)
	The abundance scatter in M33 from H II regions: is there any evidence for azimuthal metallicity variations?
o	Fig. 1, Tables 1-2: <[B2011b] NN> (Nos 1-25).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2013]
[B2013]	(Bresolin, 2013)
Write:	<<[B2013] NN>>
N:	19
Object:	Poss. HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Gemini North GMOS observations of N=19 HII region candidates in the outer disk of NGC 404.
in source:	NGC 404
Ref:	=2013ApJ...772L..23B
by	BRESOLIN F.
	Astrophys. J., 772L, 23 (2013)
	Clues on the rejuvenation of the S0 galaxy NGC 404 from the chemical abundance of its outer disk.
o	Fig. 1, Table 1: <[B2013] NN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2015]
[B2015]	(Bond, 2015)
Write:	<<[B2015] M31 BNNNA-NN>> <<[B2015] NGC 147 HII-1>>
N:	62+1
Object:	Poss. PN (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 and WFC3 observations of N=63 planetary nebula candidates in M31 and NGC 147.
in source:	M 31 = NGC 224
in source:	NGC 147
Ref:	=2015AJ....149..132B
by	BOND H.E.
	Astron. J., 149, 132 (2015)
	Hubble Space Telescope snapshot search for planetary nebulae in globular clusters of the Local Group.
o	In Table 3, FJ 4 is a probable misprint for MJ 5 (Ford M31 5 in SIMBAD).
o	Tables 2, 3, 5: <[B2015] M31 BNNNA-NN> N=62, <[B2015] NGC 147 HII-1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2017]
[B2017]	(Burenin, 2017)
Write:	<<[B2017] NNNN>>
N:	2964
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	Catalogue of N=2964 galaxy clusters detected in the Planck all-sky Compton parameter maps and identified using data from the WISE and SDSS surveys.
Ref:	=2017AstL...43..507B
by	BURENIN R.A.
	AstL, 43, 507-515 (2017)
	An extension of the Planck galaxy cluster catalogue.
o	Catalog: <[B2017] NNNN> (Nos 1-2964).
o	2017PAZh...43..559B
=E=	Catalogue in electronic form as <J/PAZh/43/559/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B2019]
[B2019]	(Bastian, 2019)= (Gaia)
Write:	<<[B2019] Gaia 8>>
N:	1
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	N=1 star cluster, from Hipparcos and Gaia DR2 data. See also [KBT2017] for seven clusters discovered in Gaia DR1 data.
Ref:	=2019A&A...630L...8B
by	BASTIAN U.
	Astron. Astrophys., 630L, 8-8 (2019)
	Gaia 8: Discovery of a star cluster containing β Lyrae.
o	<[B2019] Gaia 8> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B21]
[B21]	(Baade, 1921)
Write:	<<[B21] Leo a>> <<[B21] Vir a>>
N:	6+7
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Reference stars in the field of SW Leo and UX Vir.
Ref:	=1921AN....213..157B
by	BAADE W.
	Astron. Nachr., 213, 157-157 (1921)
	Zwei neue kurzperiodische Veraenderliche.
o	<[B21] Leo a> (Nos a-f). <[B21] Vir a> (Nos a-g).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B28]
[B28]	(Baade, 1928)
Write:	<<[B28] NNN>>
N:	114
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	ACO 1377
Ref:	=1928AN....233...65B
by	BAADE W.
	Astron. Nachr., 233, 65-72 (1928)
	Uber einen bemerkenswerten neuen Nebelhaufen in Ursa Major.
o	Table 1: <[B28] NN> N=42 among (Nos 2-57)
Ref:	=1979MNRAS.188..579B
by	BUCKNELL M.J. , GODWIN J.G., PEACH J.V.
	Mon. Not. R. Astron. Soc., 188, 579-593 (1979)
	Studies of rich clusters of galaxies- V. Photometry and luminosity functions for eight clusters.
o	Table A1: <BGP ACO 426 NNN> (Nos 1-233). Table A3: <BGP ACO 1553 NNN> (Nos 1-144). Table A4: <BGP ACO 2065 NNN> (Nos 1-156). Table A5: <BGP ACO 2147 NNN> (Nos 1-170). Table A6: <BGP ACO 2151 NNN> (Nos 1-154). Table A8: <BGP ACO 2670 NNN> (Nos 1-143). Table A2: <[B28] NNN> (Nos 60-114) added. Table A7: <[RS72] NNN> (Nos 201-272) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 3B
3B	(3rd BATSE catalog)= BATSE = (GRB)
Write:	<<3B YYMMDDA>>
N:	1122
Object:	(Gamma) (SIMBAD class: gammaBurst = Gamma-ray Burst)
Stat:	is completely incorporated in Simbad
Note:	BATSE experiment on the CGRO satellite, N=1122 cosmic gamma-ray bursts during the period 1991 April 19 to 1994 September 19. In the format 'YYMMDDA' the letters 'A', 'B', ... are added if there is more than one burst a day. (The first burst in the day is GRB YYMMDD = GRB YYMMDDA) 1999ApJS..120..399H: Information on localizatin for 218 3B bursts are obtained by analysing data from Ulysses and Compton gamma ray Observatory. see also 1B, 2B, 4B
Ref:	=1996ApJS..106...65M
by	MEEGAN C.A. , PENDLETON G.N., BRIGGS M.S., KOUVELIOTOU C., KOSHUT T.M., LESTRADE J.P., PACIESAS W.S., McCOLLOUGH M.L., BRAINERD J.J., HORACK J.M., HAKKILA J., HENZE W., PREECE R.D., MALLOZZI R.S., FISHMAN G.J.
	Astrophys. J., Suppl. Ser., 106, 65-110 (1996)
	The third BATSE γ-ray burst catalog.
o	<3B YYMMDDA> N=1122 = <Trigger NNNN>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: B3
B3	(3rd Bologna survey)= (B3.1)
Write:	<<B3 HHMM+DDdA>>
N:	13354
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	1st section of a new sky survey with the 'Northern Cross' Radiotelescope in its present version. A catalogue of 13354 radio-sources, complete to 0.1 Jy in an area of 0.78 steradian included between +37deg 15' and +47deg 37' Declination Accurate positions for 1103 sources and optical identif. for 354 sources in Vigotti 1989AJ.....98..419V
Ref:	=1985A&AS...59..255F
by	FICARRA A. , GRUEFF G., TOMASSETTI G.
	Astron. Astrophys., Suppl. Ser., 59, 255-347 (1985)
	A new Bologna sky survey at 408 MHz.
o	<B3 HHMM+DDdA>, N=13354
=E=	Catalogue in electronic form as VIII/37
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: B3.1
B3.1	(3rd Bologna survey, part 1)
*****	Avoid the usage of B3.1, prefer B3
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [B39]
[B39]	(Beyer, 1939)
Write:	<<[B39] IC 4182 a>> <<[B39] NGC 1003 a>>
N:	18+12
Object:	* (SIMBAD class: Star)
Note:	Comparison stars in the fields of IC 4182 and NGC 1003.
Ref:	=1939AN....268..341B
by	BEYER M.
	Astron. Nachr., 268, 341-354 (1939)
	Beobachtungen von Neuen Sternen.
o	Tables: <[B39] IC 4182 a> N=18 among (Nos a-w), <[B39] NGC 1003 a> N=12 among (Nos a-s).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: B3VLA
B3VLA	(B3, VLA)
Write:	<<B3VLA HHMM+DDdA>>
N:	1050
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Radio continuum data for 1050 B3 radio sources at 10.6GHz.
Ref:	=1998A&AS..133..129G
by	GREGORINI L. , VIGOTTI M., MACK K.-H., ZOENNCHEN J., KLEIN U.
	Astron. Astrophys., Suppl. Ser., 133, 129-147 (1998)
	Multi-frequency study of the B3-VLA sample. I. 10.6-GHz data.
o	Table 1: <B3VLA HHMM+DDdA> N=1050.
=E=	Catalogue in electronic form as J/A+AS/133/129
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 4B
4B	(4th BATSE catalog)= BATSE = (GRB)
Write:	<<4B YYMMDDA>>
N:	1637+1607
Object:	(Gamma) (SIMBAD class: gammaBurst = Gamma-ray Burst)
Stat:	is completely incorporated in Simbad
Note:	BATSE experiment on the CGRO satellite, N=1637 cosmic gamma-ray bursts during the period 19 April, 1991 until 29 August, 1996. Additional data have been added later, for sources until 26 May, 2000. see also 1B, 2B, 3B
Ref:	=1999ApJS..122..465P
by	PACIESAS W.S. , MEEGAN C.A., PENDLETON G.N., BRIGGS M.S., KOUVELIOTOU C., KOSHUT T.M., LESTRADE J.P., McCOLLOUGH M.L., BRAINERD J.J., HAKKILA J., HENZE W., PREECE R.D., CONNAUGHTON V., KIPPEN R.M., MALLOZZI R.S., FISHMAN G.J., RICHARDSON G.A., SAHI M.
	Astrophys. J., Suppl. Ser., 122, 465-495 (1999)
	The fourth BATSE γ-ray burst catalog (Revised).
o	<4B YYMMDDA> N=1637. <Trigger NNNN> N=1637 among (Nos 111-5586).
=E=	Catalogue in electronic form as IX/20
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [B53]
[B53]	(Brodskaja, 1953)= (Br) = (Brodskaja) = (Brodskaya)
Write:	<<[B53] NNN>>
N:	400
Object:	OB* (SIMBAD class: Star)
Note:	See also [B55b].
Ref:	=1953IzKry..10..104B
by	BRODSKAYA E.S.
	Izv. Krym. Astrofiz. Obs., 10, 104-None (1953)
	The spectra and magnitudes of 400 stars of spectral class 0-B5 in Milky Way area centered at α = 23h27m, δ = +61D.
o	Table 2: <[B53] NNN> (Nos 1-400)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B54]
[B54]	(Bidelman)= (Bi) (Not yet in Simbad)
Write:	<<[B54] NN-NNN>>
N:	1540
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Note:	In the format 'NN-NNN' the 1st 'NN' stands for the table numbering, tables (Nos 1-15)
Ref:	=1954ApJS....1..175B
by	BIDELMAN W.P.
	Astrophys. J., Suppl. Ser., 1, 175-268 (1954)
	Catalogue and bibliography of emission-line stars of types later than B.
o	Tables 1-15: objects are not in SIMBAD
o	Tables 1-15: <[B54] NN-NNN> N=1540
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B55]
[B55]	(Baade, 1955)= ([B55a])
Write:	<<[B55] N>>
N:	5
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	(Nos 1-6) No. 3 is missing
in source:	M 31 = NGC 224
Ref:	=1955AJ.....60..151B
by	BAADE W.
	Astron. J., 60, 151-151 (1955)
	Planetary nebulae in M 31.
o	<[B55] N> (Nos 1-6) (No. 3 is missing)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B55a]
[B55a]	(Baade, 1955)
*****	Avoid the usage of [B55a], prefer [B55]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B55b]
[B55b]	(Brodskaja, 1955)= (Br) = (Brodskaja) = (Brodskaya)
Write:	<<[B55b] NNNN>>
N:	5752
Object:	* (SIMBAD class: Star)
Note:	Includes stars (not all) of Brodskaja, [B53]. but the numbering is different.
Ref:	=1955IzKry..14....3B
by	BRODSKAYA E.S.
	Izv. Krym. Astrofiz. Obs., 14, 3-None (1955)
	Catalogue of spectral classes, magnitudes and color indices of 5752 stars in an area of the Milky Way centered at α = 23h25m, δ 61D30'.
o	<[B55b] NNNN> (Nos 1-5752)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B56]
[B56]	(Baade, 1956)
Write:	<<[B56] A>>
N:	3
Object:	Condensation (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=3 condensations (Nos A-C) in the jet in M 87. See also [DAF68], [PBZ99].
in source:	M 87 = NGC 4486 = Virgo A
Ref:	=1956ApJ...123..549B
by	BAADE W.
	Astrophys. J., 123, 549-551 (1956)
	Polarization in the jet of Messier 87.
o	<[B56] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B57]
[B57]	(Brun, 1957)= (Br) = (Brun) (Not yet in Simbad)
Write:	<<[B57] FFF-NNNN>>
N:	44926
Object:	* (SIMBAD class: Star)
Ref:	=1957Brun..C......0B
by	BRUN A.
	Atlas des 139 "Selected Areas" du Mt Wilson, Obs. Lyon, St Genis-Laval, 0-None (1957)
	A catalogue of 9867 stars in the Southern Hemisphere with proper motions exceeding 0".2 annually.
o	<[B57] FFF-NNNN> N=44926.
Details on Acronym: [B61]
[B61]	(Blanco)= (Bl)
Write:	<<[B61] NN>>
N:	25
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Note:	Catalogue of emission stars in the galactic center region. Identif. charts. See also PN Bl 1-A.
Ref:	=1961CoBos..13....1B
by	BLANCO V.M.
	Contr. from the Bosscha Observ. Lembang., 13, 1-11 (1961)
	A catalogue of Hα emission objects in the Galactic Center region.
o	<[B61] NN> (Nos 1-25). Table 2: <PN Bl 1-A> (Nos A-Q).
Details on Acronym: [B62]
[B62]	(Blanco, 1962)= (Blanco)
Write:	<<[B62] NN>>
N:	11
Object:	Em. Obj. (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Note:	Cepheus IV = Ass Cep OB 5
in source:	NAME Cepheus IV
Ref:	=1962PASP...74..330B
by	BLANCO V.M.
	Publ. Astron. Soc. Pac., 74, 330-332 (1962)
	Faint H-α emission objects in Cepheus IV.
o	<[B62] NN> (Nos 1-11)
Details on Acronym: [B63]
[B63]	(Bertola)
Write:	<<[B63] a>>
N:	11
Object:	* (SIMBAD class: Star)
Note:	Comparison stars in the field of NGC 3938.
Ref:	=1963MmSAI..34...33B
by	BERTOLA F.
	Mem. Soc. Astron. Ital., 34, 33-39 (1963)
	Spectrum and light curve of the supernova in NGC 3938.
o	supernova = SN 1961U
o	Table IV, Fig.4: <[B63] a> (Nos a-i, l, m).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B64]
[B64]	(Bertola)
Write:	<<[B64] NGC NNNN a>> <<[B64] Anon 0232+3725 a>>
N:	9+9+5+7+15
Object:	* (SIMBAD class: Star)
Note:	Asiago, Loiano study of supernovae. Reference stars in the field of 5 galaxies host of SN
Ref:	=1964AJ.....69..236B
by	BERTOLA F.
	Astron. J., 69, 236-242 (1964)
	Light curves of five supernovae.
o	Fig 1: <[B64] NGC 2841 a> (Nos a-i), <[B64] NGC 4374 a> (Nos a-i), <[B64] NGC 4496 a> (Nos a-e), <[B64] NGC 4382 a> (Nos a-g), <[B64] Anon 0232+3725 a> (Nos a-o).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B68]
[B68]	(Borngen, 1968)= ([B68a])
Write:	<<[B68] NN>>
N:	27
Object:	Nova (SIMBAD class: Nova = Classical Nova)
in source:	M 31 = NGC 224
Ref:	=1968AN....291...19B
by	BOERNGEN F.
	Astron. Nachr., 291, 19-24 (1968)
	Novae in M 31 auf Tautenburger Schmidt-Aufnahmen.
o	<[B68] NN> N=27
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B68a]
[B68a]	(Borngen, 1968)
*****	Avoid the usage of [B68a], prefer [B68]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B68b]
[B68b]	(Braccesi, 1968)= (B)
Write:	<<[B68b] NNN>>
N:	518
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	First quoted in 1968ApJ...152L.105B, from the 'manuscript catalogue' of Braccesi, 1968. All objects were labelled with a working number, these numbers become known as 'B' numbers. A total of 518 objects were labelled. The numbers up to 438 generally run with the RA, the others are scattered throughout the plate, and correspond to objects found in later efforts to make the survey as complete as possible.
Ref:	=1968ApJ...152L.105B
by	BRACCESI A. , LYNDS R., SANDAGE A.
	Astrophys. J., 152, 105-110 (1968)
	Spectroscopic and photometric data for a sample of Quasi-Stellar Objects identified by their infrared excess.
o	<[B68b] NNN> from the 'manuscript catalogue' of Braccesi, 1968, here N=11
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B77]
[B77]	(Bernes, 1977)= ([B77a]) = (BDN) = (Be) = (Ber) = (Bernes) = (Bs)
Write:	<<[B77] NNN>>
N:	160
Object:	HII + RFN (SIMBAD class: GalNeb = Nebula)
Ref:	=1977A&AS...29...65B
by	BERNES C.
	Astron. Astrophys., Suppl. Ser., 29, 65-70 (1977)
	A catalogue of bright nebulosities in opaque dust clouds.
o	Catalogue: <[B77] NNN> (Nos 1-160)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B77a]
[B77a]	(Bernes, 1977)
*****	Avoid the usage of [B77a], prefer [B77]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B77b]
[B77b]	(Bell, 1977)
Write:	<<[B77b] NN>>
N:	34
Object:	Knot (SIMBAD class: PartofCloud = Part of Cloud)
in source:	NAME Cas A
Ref:	=1977MNRAS.179..573B
by	BELL A.R.
	Mon. Not. R. Astron. Soc., 179, 573-586 (1977)
	Proper motions and temporal flux changes of compact features in Cassiopeia A at 5GHz.
o	Table 2: <[B77b] NN> (Nos 1-34)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B79]
[B79]	(Bartaya, 1979)= ([B79a])
Write:	<<[B79] FF DD NNN>>
N:	10396
Object:	* (SIMBAD class: Star)
Note:	In the format 'FF' stands for the SA 2 to 43, 'DD' for the declination zone, 'NNNN' is the No. of the star within the zone.
Ref:	=1979AbaOB..51....1B
by	BARTAYA R.A.
	Byull. Abastumanskaya Astrofiz. Obs., 51, 1-315 (1979)
	Catalog of spectral and luminosity classes of 10396 stars in Kapteyn's selected areas NN 2-43.
o	<[B79] FF DD NNN> N=10396
=E=	Catalogue in electronic form as III/112
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B79a]
[B79a]	(Bartaya, 1979)
*****	Avoid the usage of [B79a], prefer [B79]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B79b]
[B79b]	(Bozyan, 1979) (Not yet in Simbad)
Write:	<<[B79b] HHMM+DDd>>
N:	1049
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Table II: radio-sources with optical position coincidence, may be with more than one object. N=243 Table III: radio-sources with optical counterparts within 5 to 11 arcsec. N=102 Table IV: radio-sources with no optical counterparts within 5 to 11 arcsec. N=704 Finding charts
Ref:	=1979AJ.....84..910B
by	BOZYAN E.P.
	Astron. J., 84, 910-941 (1979)
	Position coincidence optical identifications using Texas interferometer radio positions.
o	Tables II, III, IV: <[B79b] HHMM+DDd> N=243+102+704
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B79c]
[B79c]	(Beichman, 1979)= (IRS)
Write:	<<[B79c] AFGL 4029 IRS N>>
N:	2
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	In Beichman Thesis, 1979, N=2 main sources of 10-20microm emission in the region of AFGL 4029.
Ref:	=2001RMxAA..37...83Z
by	ZAPATA L.A. , RODRIGUEZ L.F., KURTZ S.E.
	Rev. Mex. Astron. Astrofis., 37, 83-86 (2001)
	A subarcsecond radio binary associated with AFGL 4029-IRS1.
o	IRS sources from Beichman Thesis, 1979.
o	<[B79c] AFGL 4029 IRS N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B80]
[B80]	(Baier, 1980)= (Anon)
Write:	<<[B80] Anon N>>
N:	4
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
in source:	NAME UMA SUPERCL
Ref:	=1980AN....301...17B
by	BAIER F.W.
	Astron. Nachr., 301, 17-26 (1980)
	Investigation of galaxy distribution in the Ursa Major supercluster of galaxies.
o	Table I: <[B80] Anon N> (Nos 1-4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B81]
[B81]	(Bally, 1981)= (IRS)
Write:	<<[B81] Sh 2-87 IRS N>>
N:	1
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	From Bally J., 1981, Ph.D. Thesis, Univ. of Massachusetts at Amherst.
in source:	SH 2-87
Ref:	=1989ApJ...345..268B
by	BARSONY M.
	Astrophys. J., 345, 268-281 (1989)
	A close-up view of the S87 molecular outflow.
o	[B81] Sh 2-87 IRS 1 from Bally J., 1981, Ph.D. Thesis.
o	Text: <[B81] Sh 2-87 IRS N> (No. 1). Fig.1: <[B89] knot A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B82]
[B82]	(Brosch, 1982)
Write:	<<[B82] A>>
N:	5
Object:	Unknown (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	A ring galaxy found on a PSS plate, near SAO 44762.
Ref:	=1982A&A...112..388B
by	BROSCH N.
	Astron. Astrophys., 112, 388-390 (1982)
	A new ring galaxy in Canes Venatici.
o	Table 1: <[B82] A> (Nos A-D, K).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B84]
[B84]	(Blanco, 1984)= (Blanco) = (BW)
Write:	<<[B84] NN>> <<[B84] ENN>>
N:	81+12
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	(Nos 1-81) and (Nos E1-E12) E for Eclipsing variables
Ref:	=1984AJ.....89.1836B
by	BLANCO B.M.
	Astron. J., 89, 1836-1868 (1984)
	RR Lyrae variables in Baade's window.
o	Cross-id. G (Gaposchkin) not in Simbad
o	<[B84] NN> N=81, <[B84] ENN> N=12
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B86]
[B86]	(Blanco, 1986)= ([B86a]) = (Bla)
Write:	<<[B86] NNN>>
N:	174
Object:	M Giant (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1986AJ.....91..290B
by	BLANCO V.M.
	Astron. J., 91, 290-292 (1986)
	Giants of type M1 or later in Baade's window.
o	<[B86] NNN> (Nos 1-174)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B86a]
[B86a]	(Blanco, 1986)
*****	Avoid the usage of [B86a], prefer [B86]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B86b]
[B86b]	(Bergeron, 1986)
Write:	<<[B86b] NN>>
N:	15
Object:	G (SIMBAD class: Galaxy)
Note:	Table 1: N=15 galaxies in the field of the QSO PKS 2128-12 See also [BB86b], [BDK87], [B88], [BBK88], [BB91], [BCS92], [GB97]
Ref:	=1986A&A...155L...8B
by	BERGERON J.
	Astron. Astrophys., 155, 8-11 (1986)
	The Mg II absorption system in the QSO PKS 2128-12 : a galaxy disc/halo with a radius of 65 kpc.
o	Table 1: <B86b] NN> (Nos 1-15)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B86c]
[B86c]	(Blecha, 1986)= (B)
Write:	<<[B86c] NN>>
N:	33
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	N=33 globular cluster candidates in NGC 253. See also [LA83], [BS2000].
in source:	NGC 253
Ref:	=1986A&A...154..321B
by	BLECHA A.
	Astron. Astrophys., 154, 321-335 (1986)
	Search for the globular clusters in nearby galaxies. I. NGC 253.
o	Table 3: <[B86c] NN> (Nos 1-33).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B87]
[B87]	(Brown, 1987)= (R) = (VLA)
Write:	<<[B87] NN>>
N:	11
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
in source:	NAME R CrA Cloud
Ref:	=1987ApJ...322L..31B
by	BROWN A.
	Astrophys. J., 322, 31-34 (1987)
	Radio emission from pre-main-sequence stars in Corona Australis.
o	[TS84] IRS 7 = [BZ75] R CrA 1
o	Table 1: <[B87] NN> (Nos 1-11), Table 2: <[TS84] IRS NNA> (Nos 7A, 7B)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B88]
[B88]	(Bergeron, 1988)= ([B88a])
Write:	<<[B88] HHMM+DD G1>>
N:	13
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Table 4: N=13 galaxies associated with 13 QSO. We use the format of the QSO 'HHMM+DD' and we add 'G1' to distinguish the galaxy from the QSO. See also [B86b], [BB86b], [BDK87], [BBK88], [BB91], [BCS92], [GB97]
Ref:	=1988IAUS..130..343B
by	BERGERON J.
	130th Symposium of the IAU held in Balatonfured, Hungary, June 15-20, 1987. Ed. by J. Audouze, M.C. Pelletan and A. Szalay. Large scale structures of the universe., 130, 343-358 (1988)
	Galaxies giving rise to MgII absorption systems in quasar spectra.
o	Table 4: <[B88] HHMM+DD G1> N=13
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B88a]
[B88a]	(Bergeron, 1988)
*****	Avoid the usage of [B88a], prefer [B88]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B88b]
[B88b]	(Buta, 1988)
Write:	<<[B88b] NGC4725 NN>>
N:	10
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	AAT MarkII and TAURUS Fabry-Perot interferometer Halpha observations. N=10 HII regions in the inner ring of NGC 4725.
in source:	NGC 4725
Ref:	=1988ApJS...66..233B
by	BUTA R.
	Astrophys. J., Suppl. Ser., 66, 233-259 (1988)
	The structure and dynamics of ringed galaxies. V. The kinematics of NGC 1512, NGC 3351, NGC 4725, and NGC 4736.
o	Table 4: <[B88b] NGC4725 NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B89]
[B89]	(Barsony, 1989)
Write:	<<[B89] knot A>>
N:	2
Object:	Knot (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
in source:	SH 2-87
Ref:	=1989ApJ...345..268B
by	BARSONY M.
	Astrophys. J., 345, 268-281 (1989)
	A close-up view of the S87 molecular outflow.
o	[B81] Sh 2-87 IRS 1 from Bally J., 1981, Ph.D. Thesis.
o	Text: <[B81] Sh 2-87 IRS N> (No. 1). Fig.1: <[B89] knot A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B90]
[B90]	(Braun, 1990)= ([B90a])
Write:	<<[B90] NNN>>
N:	534
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
in source:	M 31 = NGC 224
Ref:	=1990ApJS...72..761B
by	BRAUN R.
	Astrophys. J., Suppl. Ser., 72, 761-775 (1990)
	The interstellar medium of M 31. II. A survey of 20 centimeter continuum emission.
o	Table 2: <[B90] NNN> N=534
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B90a]
[B90a]	(Braun, 1990)
*****	Avoid the usage of [B90a], prefer [B90]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B90b]
[B90b]	(Block, 1990) (Not yet in Simbad)
Write:	<<[B90b] N>>
N:	2
Object:	Cometary Globule (SIMBAD class: ComGlob = Cometary Globule / Pillar)
Note:	Object 1 = IRAS 06314+0427, Object 2 = AFGL 961
in source:	NAME Rosette Nebula
Ref:	=1990Natur.347..452B
by	BLOCK D.L.
	Nature, 347, 452-None (1990)
	A family of cometary globules around an infrared source near the Rosette nebula.
o	<[B90b] N> (Nos 1-2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B91]
[B91]	(Battinelli, 1991)= ([B91a]) = (B-0B) = (OB) = (SMC OB)
Write:	<<[B91] NN>>
N:	31
Object:	OB Assoc. (SIMBAD class: Association = Association of Stars)
Stat:	is completely incorporated in Simbad
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1991A&A...244...69B
by	BATTINELLI P.
	Astron. Astrophys., 244, 69-74 (1991)
	A new identification technique for OB associations: OB associations in the Small Magellanic Cloud.
o	<[B91] NN> (Nos 1-31)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B91a]
[B91a]	(Battinelli, 1991)
*****	Avoid the usage of [B91a], prefer [B91]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B91b]
[B91b]	(Birkle, 1991)
Write:	<<[B91b] HHMMSS+DDMM.m>>
N:	1
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Stat:	is completely incorporated in Simbad
Note:	Calar Alto observations. Discovery of a probable nova in M 31.
in source:	M 31 = NGC 224
Ref:	=1991IAUC.5213....1B
by	BIRKLE K.
	IAU Circ., 5213, 1-None (1991)
	Nova in M 31.
o	<[B91b] HHMMSS+DDMM.m> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B92a]
[B92a]	(Bhatia, 1992)
Write:	<<[B92a] NN>>
N:	10
Object:	Pair of Cl (SIMBAD class: Blend = Composite Object, Blend)
Stat:	is completely incorporated in Simbad
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1992MmSAI..63..141B
by	BHATIA R.K.
	Mem. Soc. Astron. Ital., 63, 141-144 (1992)
	Integrated CCD photometry of binary clusters in the Large Magellanic Cloud.
o	<[B92a] NN> N=10
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B92b]
[B92b]	(Burton, 1992)
Write:	<<[B92b] NN>>
N:	30 among 37
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
in source:	NAME R CrA Cloud
Ref:	=1992PASAu..10...52B
by	BURTON M.
	Proc. Astron. Soc. Australia, 10, 52-54 (1992)
	An infrared imaging survey of the ρ Oph and R CrA darkcloud cores.
o	Table 1: <[B92b] NN> N=30 among (Nos 1-37).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B93]
[B93]	(Binggeli, 1993)
Write:	<<[B93] NN>>
N:	40
Object:	Dwarf G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-41) dwarf galaxies first numbered by Binggeli, 1993, 'Dwarf galaxies as bound companions', Habilitationsschrift, University of Basel, Switzerland. This numbering is used by Van Driel+ in 1998A&AS..127..397V and 1998A&AS..129..313B See also [VKB98] [B93] galaxies with no previously known identification are called 'Anon N' in 1998A&AS..127..397V, '[VKB98] Anon N' in SIMBAD.
in source:	NAME M 81 GROUP
Ref:	=1998A&AS..127..397V
by	VAN DRIEL W. , KRAAN-KORTEWEG R.C., BINGGELI B., HUCHTMEIER W.K.
	Astron. Astrophys., Suppl. Ser., 127, 397-408 (1998)
	An HI line search for optically identified dwarf galaxy candidates in the M 81 group.
o	Table 1, col.1: <[B93] NN> (Nos 1-41), No. 5 missing. Table 1, col.2: <[VKB98] Anon N> (Nos 1-7). Table 1, col.2: <K68 NNNW> (Nos 1N-8N).
Ref:	=1998A&AS..129..313B
by	BREMNES T. , BINGGELI B., PRUGNIEL P.
	Astron. Astrophys., Suppl. Ser., 129, 313-328 (1998)
	Structure and stellar content of dwarf galaxies. I. B and R photometry of dwarf galaxies in the M 81 group.
o	Table 1: <[B93] NN> (Nos 1-41)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B94]
[B94]	(Bird, 1994)
Write:	<<[B94] Clump A>>
N:	4
Object:	Subcluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=4 clumps or subclusters in ACO 2670.
in source:	ACO 2670
Ref:	=1994ApJ...422..480B
by	BIRD C.
	Astrophys. J., 422, 480-485 (1994)
	Substructure in clusters and cD peculiar velocities: A 2670.
o	cD galaxy = [SEG88] 1.
o	Table 1: <[B94] Clump A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: B96
B96	(Barger+, 1996)
*****	Avoid the usage of B96, prefer [BAE96]
Origin	of the Acronym: L (1998ApJ...497..188C)
Details on Acronym: [B96]
[B96]	(Bontemps, 1996)
Write:	<<[B96] LNNNN N>> <<[B96] LNNNNA N>> <<[B96] LNNNNWN N>> <<[B96] B217 N>> <<[B96] TMC-2A N>> <<[B96] Ori-I-2 N>> <<[B96] LBSNN N>> <<[B96] TDR12 N>> <<[B96] OphB2 N>> <<[B96] OphF N>> <<[B96] Serpens NN>>
N:	64
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	From Bontemps S. Thesis, 1996. N=64 VLA sources detected in 19 regions. See also [BAW95], OphB2.
Auth.:	BONTEMPS S.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B97a]
[B97a]	(Blakeslee, 1997) (Not yet in Simbad)
Write:	<<[B97a] ACO NNNN-N>>
N:	23
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	N=23 brightest galaxies in 19 ACO clusters (BCG)
Ref:	=1997ApJ...481L..59B
by	BLAKESLEE J.P.
	Astrophys. J., 481, 59-62 (1997)
	The dependence of globular cluster number on density for Abell cluster central galaxies.
o	Table 1: <[B97a] ACO NNNN-N> N=23
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B97b]
[B97b]	(Balcells, 1997)= (Dw)
Write:	<<[B97b] Dw N>>
N:	2
Object:	Dwarf G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
in source:	NGC 3656
Ref:	=1997ApJ...486L..87B
by	BALCELLS M.
	Astrophys. J., 486, 87-90 (1997)
	Two tails in NGC 3656 and the major merger origin of shell and minor-axis dust lane elliptical galaxies.
o	<[B97b] Dw N> (Nos 1-2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B98]
[B98]	(Beck-Winchatz, 1998)= ([B98a])
Write:	<<[B98] NN>>
N:	10
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Note:	Table 4: N=10 QSO candidates from Beck-Winchatz thesis, 1998 Tables 1-3: [BA99] QSO candidates.
Ref:	=1999AJ....117.2582B
by	BECK-WINCHATZ B. , ANDERSON S.F.
	Astron. J., 117, 2582-2593 (1999)
	A morphological and multicolor survey for faint QSOs in the Groth-Westphal strip.
o	Tables 1, 2, 3: <[BA99] NNNN> N=20 among (Nos 72-1702). Table 4: <[B98] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B98a]
[B98a]	(Beck-Winchatz, 1998)
*****	Avoid the usage of [B98a], prefer [B98]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B98b]
[B98b]	(Becker, 1998) (Not yet in Simbad)
Write:	<<[B98b] NN>>
N:	7
Object:	Knot (SIMBAD class: PartofCloud = Part of Cloud)
Note:	ROSAT, ASCA and BepoSAX observations. (Nos N1-N7), 7 brightest compact knots in RCW 89.
in source:	RCW 89
Ref:	=1998MmSAI..69..847B
by	BECKER W.
	Mem. Soc. Astron. Ital., 69, 847-855 (1998)
	X-ray emission characteristics of rotation-powered pulsars and their wind nebulae.
o	Fig.1: <[B98b] AN> (Nos N1-N7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B99]
[B99]	(Burbidge, 1999)= ([B99a])
Write:	<<[B99] JHHMM+DDMM>>
N:	14
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	QSO near NGC 1068.
Ref:	=1999ApJ...511L...9B
by	BURBIDGE E.M.
	Astrophys. J., 511, 9-11 (1999)
	A group of quasi-stellar objects closely associated with NGC 1068.
o	Table 2: Objects 'ROSAT counts' are [R97] NGC 1068 NN.
o	Table 2: <[B99] JHHMM+DDMM> N=14.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B99a]
[B99a]	(Burbidge, 1999)
*****	Avoid the usage of [B99a], prefer [B99]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [B99b]
[B99b]	(Bhatt, 1999)
Write:	<<[B99b] NN>>
N:	16
Object:	* (SIMBAD class: Star)
Note:	N=16 stars in the field of CG 30-CG 31 Complex. Map in Fig.1.
Ref:	=1999MNRAS.308...40B
by	BHATT H.C.
	Mon. Not. R. Astron. Soc., 308, 40-44 (1999)
	Magnetic fields in cometary globules - II. CG 30-31 complex.
o	Table 1: <[B99b] NN> (Nos 1-16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BA
BA	(Baade+Arp)= (B)
Write:	<<BA 1-NNN>> <<BA 2-NN>> <<BA 3-NN>> <<BA 4-NN>>
N:	688+68+30+40
Object:	Em. Nebula + Exgl Nebula + GCl + Misc. Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
in source:	M 31 = NGC 224
Ref:	=1964ApJ...139.1027B
by	BAADE W. , ARP H.C.
	Astrophys. J., 139, 1027-1044 (1964)
	Positions of emission nebulae in M 31.
o	Table 1: <BA 1-NNN> N=688, Table 2: <BA 2-NN> N=68, Table 3: <BA 3-NN> N=30, Table 4: <BA 4-NN> N=40.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BA
BA	(Balloon number)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ba
ba	(Balogh+)
*****	Avoid the usage of ba, prefer [BBS2002]
Origin	of the Acronym: L (2008A&A...486....9V)
Details on Acronym: Ba
Ba	(Basel astr. institute)
*****	Avoid the usage of Ba, prefer Basel
Details on Acronym: Ba
Ba	(Baade)
Write:	<<PN Ba N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Ba 1 = PN G171.3-25.8 = PK 171-25 1
Ref:	=1935PASP...47...99B
by	BAADE W.
	Publ. Astron. Soc. Pac., 47, 99-None (1935)
	A new planetary nebula.
o	<PN Ba 1>.
Details on Acronym: [BA2007]
[BA2007]	(Beck-Winchatz+Anderson, 2007)
Write:	<<[BA2007] NNN>>
N:	15+31+3
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Note:	Use of archival HST WFPC2 images of several fields to search for QSO candidates. See also [BA99].
Ref:	=2007MNRAS.374.1506B
by	BECK-WINCHATZ B. , ANDERSON S.F.
	Mon. Not. R. Astron. Soc., 374, 1506-1514 (2007)
	Faint quasar candidates from Hubble Space Telescope imaging: number counts from 31 new high-latitude fields.
o	Tables 2,3,4: <[BA2007] NNN> N=15+31+3 among (Nos 1-391).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ba87
Ba87	(Battistini+, 1987)
*****	Avoid the usage of Ba87, prefer Bol
Origin	of the Acronym: L (2001A&A...373...63S)
Details on Acronym: [BA97]
[BA97]	(Bontemps+Andre, 1997) (Not yet in Simbad)
Write:	<<[BA97] A>>
N:	3
Object:	(Radio) (SIMBAD class: Radio = Radio Source)
Note:	VLA 3.6cm observations of N=3 radio knots in the field of NAME VLA 1623-243.
in source:	NAME VLA 1623-243
Ref:	=1997IAUS..182P..63B
by	BONTEMPS S. , ANDRE P.
	IAUS, 182P, 63-65 (1997)
	An asymmetric radio continuum HH-jet from VLA1623.
o	Fig. 1: <[BA97] A> (Nos A-C).
Details on Acronym: [BA99]
[BA99]	(Beck-Winchatz+Anderson, 1999)
Write:	<<[BA99] NNNN>>
N:	20
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Note:	HST WFPC2 observations. Tables 1-3: N=20 QSO candidates from the authors' catalogue. Table 3: UV compact objects. Table 4: [B98] QSO candidates from Beck-Winchatz thesis. See also [BA2007].
Ref:	=1999AJ....117.2582B
by	BECK-WINCHATZ B. , ANDERSON S.F.
	Astron. J., 117, 2582-2593 (1999)
	A morphological and multicolor survey for faint QSOs in the Groth-Westphal strip.
o	Tables 1, 2, 3: <[BA99] NNNN> N=20 among (Nos 72-1702). Table 4: <[B98] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BAaDE
BAaDE	(Bulge Asymmetries and Dynamical Evolution)
Write:	<<BAaDE aa3a-NNNNN>>
N:	28062
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	The Bulge Asymmetries and Dynamical Evolution (BAaDE) survey consists of N=28062 sources selected by MSX colors. The survey covers the full Galactic plane, utilizing both the Karl G. Jansky Very Large Array (VLA) at 43 GHz and the Atacama Large Millimeter/submillimeter Array (ALMA) at 86 GHz. For more information, visit: http://www.phys.unm.edu/~baade/
in source:	NAME Galactic Bulge
Ref:	=2018ApJ...862..153S
by	STROH M.C. , PIHLSTROM Y.M., SJOUWERMAN L.O., CLAUSSEN M.J., MORRIS M.R., RICH M.R.
	Astrophys. J., 862, 153-153 (2018)
	Quasi-simultaneous 43 and 86 GHz SiO maser observations and potential bias in the BAaDE survey are resolved.
o	Tables 2-3: <BAaDE aa3a-NNNNN> N=86.
Ref:	=2019ApJS..244...25S
by	STROH M.C. , PIHLSTROM Y.M., SJOUWERMAN L.O., LEWIS M.O., CLAUSSEN M.J., MORRIS M.R., RICH R.M.
	Astrophys. J., Suppl. Ser., 244, 25-25 (2019)
	The Bulge Asymmetries and Dynamical Evolution (BAaDE) SiO maser survey at 86 GHz with ALMA.
o	Tables 2+5: <BAaDE aa3a-NNNNN> N=1427+4.
Ref:	=2020ApJ...892...52L
by	LEWIS M.O. , PIHLSTROM Y.M., SJOUWERMAN L.O., STROH M.C., MORRIS M.R., (The BAaDE Collaboration)
	Astrophys. J., 892, 52-52 (2020)
	Carbon- and Oxygen-rich Asymptotic Giant Branch (AGB) stars in the Bulge Asymmetries and Dynamical Evolution (BAaDE) survey.
o	Tables 1-3: <BAaDE aa3a-NNNNN> N=6+23+33.
Ref:	=2020ApJ...901...98L
by	LEWIS M.O. , PIHLSTROM Y.M., SJOUWERMAN L.O., QUIROGA-NUNEZ L.H.
	Astrophys. J., 901, 98-98 (2020)
	Infrared color separation between thin-shelled oxygen-rich and carbon-rich AGB stars.
o	Tables 1-2: <BAaDE aa3a-NNNNN> N=7+44.
Ref:	=2021AJ....161..111D
by	DIKE V. , MORRIS M.R., RICH R.M., LEWIS M.O., QUIROGA-NUNEZ L.H., STROH M.C., TRAPP A.C., CLAUSSEN M.J.
	Astron. J., 161, 111-111 (2021)
	Ground vibrational state SiO emission in the VLA BAaDE survey.
o	Table 1: <BAaDE aa3a-NNNNN> N=90.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Baade
Baade	(Baade)
*****	Avoid the usage of Baade, prefer [SN45]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Baade Swope
Baade Swope	(Baade+Swope)
*****	Avoid the usage of Baade Swope, prefer BASV
Details on Acronym: [BAB2001]
[BAB2001]	(Brotherton+Arav+Becker+, 2001)
Write:	<<[BAB2001] JHHMM+DDMM>>
N:	1
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	Discovery of a bright QSO, 'J2359-1241' associated with the radio-source NVSS J235953-124148.
Ref:	=2001ApJ...546..134B
by	BROTHERTON M.S. , ARAV N., BECKER R.H., TRAN H.D., GREGG M.D., WHITE R.L., LAURENT-MUEHLEISEN S.A., HACK W.
	Astrophys. J., 546, 134-139 (2001)
	QSO 2359-1241: a bright, highly polarized, radio-moderate, reddened, low-ionization broad absorption line quasar.
o	QSO J2359-1241 = [BAB2001] J2359-1241
o	<[BAB2001] J2359-1241> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAB2002]
[BAB2002]	(Bauer+Alexander+Brandt+, 2002)
Write:	<<[BAB2002] N>>
N:	6
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations. N=6 extended X-ray sources in the CDFN.
in source:	NAME CDFN
Ref:	=2002AJ....123.1163B
by	BAUER F.E. , ALEXANDER D.M., BRANDT W.N., HORNSCHEMEIER A.E., MIYAJI T., GARMIRE G.P., SCHNEIDER D.P., BAUTZ M.W., CHARTAS G., GRIFFITHS R.E., SARGENT W.L.W.
	Astron. J., 123, 1163-1178 (2002)
	The Chandra Deep Field North survey. IX. Extended X-ray sources.
o	ClG 1236+6215 is ClG J1236+6215
o	Table 1: <[BAB2002] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAB2009]
[BAB2009]	(Beirao+Appleton+Brandl+, 2009)
Write:	<<[BAB2009] A>>
N:	8
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Palomar 60" optical, Palomar 200" WIRC NIR, Spitzer mid-IR and GALEX UV observations of the interacting galaxy system Arp 143.
in source:	APG 143
Ref:	=2009ApJ...693.1650B
by	BEIRAO P. , APPLETON P.N., BRANDL B.R., SEIBERT M., JARRETT T., HOUCK J.R.
	Astrophys. J., 693, 1650-1665 (2009)
	Powerful H_{2} emission and star formation on the interacting galaxy system Arp 143: observations with Spitzer and GALEX.
o	Table 4, Fig. 2: <[BAB2009] A> (Nos A-H).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAB2010]
[BAB2010]	(Bally+Aguirre+Battersby+, 2010) (Not yet in Simbad)
Write:	<<[BAB2010] GLLL.ll+BB.bb>>
N:	40
Object:	mm clump (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	Caltech Submillimeter Observatory Bolocam and SHARC-II 1.1mm observations of N=40 clumps in the Galactic center region.
in source:	NAME Galactic Center
Ref:	=2010ApJ...721..137B
by	BALLY J. , AGUIRRE J., BATTERSBY C., BRADLEY E.T., CYGANOWSKI C., DOWELL D., DROSBACK M., DUNHAM M.K., EVANS II N.J., GINSBURG A., GLENN J., HARVEY P., MILLS E., MERELLO M., ROSOLOWSKY E., SCHLINGMAN W., SHIRLEY Y.L., STRINGFELLOW G.S., WALAWENDER J., WILLIAMS J.
	Astrophys. J., 721, 137-163 (2010)
	The Bolocam Galactic Plane Survey: λ = 1.1 and 0.35 mm dust continuum emission in the Galactic Center region.
o	Table 2: <[BAB2010] GLLL.ll+BB.bb> N=40.
=E=	Catalogue in electronic form as J/ApJ/721/137
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAB2012]
[BAB2012]	(Bania+Anderson+Balser, 2012)
Write:	<<[BAB2012] GNN>> <<[BAB2012] G52L>>
N:	2+1
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Arecibo radio recombination line observations of N=3 HII regions. Use of Spitzer MIPSGAL and GLIMPSE data.
Ref:	=2012ApJ...759...96B
by	BANIA T.M. , ANDERSON L.D., BALSER D.S.
	Astrophys. J., 759, 96 (2012)
	The Arecibo H II Region Discovery Survey.
o	Fig. 1, Table 1: <HRDS GLLL.lll+BB.bbb> N=37. Paragr. 6.3 and 6.4: <[BAB2012] GNN> (Nos G46, G52), <[BAB2012] G52L> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAB2014]
[BAB2014]	(Bouy+Alves+Bertin+, 2014)
Write:	<<[BAB2014] NNNNNN>>
N:	605020
Object:	* (SIMBAD class: Star)
Note:	CTIO Blanco telescope DECam observations of N=605020 sources in a field of about 10 square degrees of the sky, centered on NGC 1980.
in source:	NAME ORI A MCLD
Ref:	=2014A&A...564A..29B
by	BOUY H. , ALVES J., BERTIN E., SARRO L.M., BARRADO D.
	Astron. Astrophys., 564A, 29-29 (2014)
	Orion revisited. II. The foreground population to Orion A.
o	Table A.1: <[BAB2014] NNNNNN> (Nos 1-605020).
o	Fig. 4 Group 189 not identified.
=E=	Catalogue in electronic form as <J/A+A/564/A29/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAB2017]
[BAB2017]	(Bellini+Anderson+Bedin+, 2017)
Write:	<<[BAB2017] NNNNNN>>
N:	478477
Object:	* (SIMBAD class: Star)
Note:	N=478477 stars in the core of ω Centauri. Use of HST WFC3 archival data. See also [BLB2018] for stars in one parallel HST field.
in source:	NGC 5139 = ome Cen
Ref:	=2017ApJ...842....6B
by	BELLINI A. , ANDERSON J., BEDIN L.R., KING I.R., VAN DER MAREL R.P., PIOTTO G., COOL A.
	Astrophys. J., 842, 6-6 (2017)
	The state-of-the-art HST astro-photometric analysis of the core of ω Centauri. I. The catalog.
o	Table 3: <[BAB2017] NNNNNN> (Nos 1-478477).
=E=	Catalogue in electronic form as <J/ApJ/842/6/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BAC
BAC	(Bordeaux Astrographic Catalogue)= (Bor-AC)
Write:	<<NAME BAC NNN>>
Object:	* (SIMBAD class: Star)
=E=	Catalogue in electronic form as I/228
Details on Acronym: [BAC2008]
[BAC2008]	(BOumis+Alikakos+Christopoulou+, 2008)
Write:	<<[BAC2008] AN>>
N:	7
Object:	Filament (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Skinakas Observatory 0.3m telescope images of SNR 15.1-1.6.
in source:	SNR G015.1-01.6
Ref:	=2008A&A...481..705B
by	BOUMIS P. , ALIKAKOS J., CHRISTOPOULOU P.E., MAVROMATAKIS F., XILOURIS E.M., GOUDIS C.D.
	Astron. Astrophys., 481, 705-712 (2008)
	First optical detection of the supernova remnant G 15.1-1.6.
o	Fig.1, Text: <[BAC2008] AN> (Nos A, B, C1-C2, E1-E2, F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAC2016]
[BAC2016]	(Barbosa+Arnaboldi+Coccato+, 2016) (Not yet in Simbad)
Write:	<<[BAC2016] {cen\|inn\|out}N{s}NNa>>
N:	119
Object:	Star (SIMBAD class: Star)
Note:	VLT FORS2 observations of N=119 stars in NGC 3311, at the centre of the Hydra I cluster. The six masks that sample the stellar halo in shells are: cen1, cen2, inn1, inn2, out1, and out2.
in source:	NAME Hya I Cluster: NGC 3311 = NGC 3311
Ref:	=2016A&A...589A.139B
by	BARBOSA C.E. , ARNABOLDI M., COCCATO L., HILKER M., MENDES DE OLIVEIRA C., RICHTLER T.
	Astron. Astrophys., 589A, 139-139 (2016)
	The Hydra I cluster core. I. Stellar populations in the cD galaxy NGC 3311.
o	Table 1: <[BAC2016] cenNsNNa> N=42, <[BAC2016] innNsNNa> N=38, <[BAC2016] outNsNNa> N=39.
=E=	Catalogue in electronic form as <J/A+A/589/A139/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Bad
Bad	(Badaljan)= (Badalian) = (Badaljan)
Write:	<<Bad NN>>
N:	35
Object:	V* (SIMBAD class: Variable* = Variable Star)
Ref:	=1960DoArm..31..261B
by	BADALJAN G.S.
	Doklady - Akad. Nauk Arm. SSR, 31, 261-266 (1960)
	Uber eine Gruppe veranderlich-verdachtiger Sterne vom T Tauri-Typ.
o	Table 1: <Bad NN> (Nos 1-35).
Origin	of the Acronym: L (2002A&A...383..598M)
Details on Acronym: [BAD2001]
[BAD2001]	(Bond+Abe+Dodd+, 2001)= (MOA)
Write:	<<[BAD2001] ngbNN-N-NNNN>>
N:	25
Object:	Poss. Microlensing Event (SIMBAD class: LensingEv = (Micro)Lensing Event)
Stat:	is completely incorporated in Simbad
Note:	Observations of the Galactic Bulge by the MOA group. See also [SAB2003].
in source:	NAME Galactic Bulge
Ref:	=2001MNRAS.327..868B
by	BOND I.A. , ABE F., DODD R.J., HEARNSHAW J.B., HONDA M., JUGAKU J., KILMARTIN P.M., MARLES A., MASUDA K., MATSUBARA Y., MURAKI Y., NAKAMURA T., NANKIVELL G., NODA S., NOGUCHI C., OHNISHI K., RATTENBURY N.J., REID M., SAITO T., SATO H., SEKIGUCHI M., SKULJAN J., SULLIVAN D.J., SUMI T., TAKEUTI M., WATASE Y., WILKINSON S., YAMADA R., YANAGISAWA T., YOCK P.C.M.
	Mon. Not. R. Astron. Soc., 327, 868-880 (2001)
	Real-time difference imaging analysis of MOA Galactic bulge observations during 2000.
o	Tables 1, 4: <[BAD2001] ngbNN-N-NNN> N=25.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAD2016]
[BAD2016]	(Bouwens+Aravena+Decarli+, 2016)
Write:	<<[BAD2016] AAAA-NNNNNNNNNN>>
N:	45
Object:	G (SIMBAD class: Galaxy)
Note:	ALMA Band 6 observations of N=45 galaxies at z<4 within the region of the HUDF. Use of the ALMA SPECtroscopic Survey in the Hubble Ultra-Deep Field (ASPECS). See also [BIO2015].
in source:	NAME Hubble Ultra Deep Field
Ref:	=2016ApJ...833...72B
by	BOUWENS R.J. , ARAVENA M., DECARLI R., WALTER F., DA CUNHA E., LABBE I., BAUER F.E., BERTOLDI F., CARILLI C., CHAPMAN S., DADDI E., HODGE J., IVISON R.J., KARIM A., LE FEVRE O., MAGNELLI B., OTA K., RIECHERS D., SMAIL I.R., VAN DER WERF P., WEISS A., COX P., ELBAZ D., GONZALEZ-LOPEZ J., INFANTE L., OESCH P., WAGG J., WILKINS S.
	Astrophys. J., 833, 72-72 (2016)
	ALMA spectroscopic survey in the Hubble Ultra Deep Field: the infrared excess of UV-selected z = 2-10 galaxies as a function of UV-continuum slope and stellar mass.
o	Tables 3-4, 10: <[BAD2016] AAAA-NNNNNNNNNN> N=45.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Badalian
Badalian	(Badaljan)
*****	Avoid the usage of Badalian, prefer Bad
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Badaljan
Badaljan	(Badaljan)
*****	Avoid the usage of Badaljan, prefer Bad
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BAE2000]
[BAE2000]	(Brosch+Almoznino+Engels+, 2000)
Write:	<<[BAE2000] NN>>
N:	75
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	N=75 FAUST sources and counterparts.
in source:	NAME NGP
Ref:	=2000MNRAS.316...58B
by	BROSCH N. , ALMOZNINO E., ENGELS D., BOWYER S., LAMPTON M.
	Mon. Not. R. Astron. Soc., 316, 58-70 (2000)
	FAUST observations near the North Galactic Pole.
o	Table 1: <[BAE2000] NN> (Nos 1-75).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAE2005]
[BAE2005]	(Belokurov+An+Evans+, 2005)
Write:	<<[BAE2005] NN N>>
N:	3+3+16
Object:	Poss. Lensing Event + V* (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	AGAPE survey: Search for microlensing events in M 31: results in terms of 3 levels candidates: N=3 candidates at level 1 (the most trustworthy), N=3 candidates at level 2, At level 3, 16 candidates are identified as varible stars. In the format the first digits 'NN' stand for candidates, the second part 'N' stands for the level. See also AGAPE.
in source:	M 31 = NGC 224
Ref:	=2005MNRAS.357...17B
by	BELOKUROV V. , AN J., EVANS N.W., HEWETT P., BAILLON P., CALCHI NOVATI S., CARR B.J., CREZE M., GIRAUD-HERAUD Y., GOULD A., JETZER P., KAPLAN J., KERINS E., PAULIN-HENRIKSSON S., SMARTT S.J., STALIN C.S., TSAPRAS Y., WESTON M.J.
	Mon. Not. R. Astron. Soc., 357, 17-37 (2005)
	The POINT-AGAPE survey - II. An unrestricted search for microlensing events towards M31.
o	Tables 3, 4, 6: <[BAE2005] NN N> N=3+3+16.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAE96]
[BAE96]	(Barger+Aragon-Salamanca+Ellis+, 1996)= (B96)
Write:	<<[BAE96] AC NNN NNN>>
N:	92+117+120
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	ACCG 114 = ACO S 1077
in source:	ACCG 118 = ACO 2744
in source:	ACCG 103 = ACO S 910
Ref:	=1996MNRAS.279....1B
by	BARGER A.J. , ARAGON-SALAMANCA A., ELLIS R.S., COUCH W.J., SMAIL I., SHARPLES R.M.
	Mon. Not. R. Astron. Soc., 279, 1-24 (1996)
	The life-cycle of star formation in distant clusters.
o	AC 114, 118, 103 = ACCG 114, 118, 103
o	Table 4: <[BAE96] AC 114 NNN> N=92 among (Nos 2-188), Table 5: <[BAE96] AC 118 NNN> N=117 among (Nos 2-197), Table 6: <[BAE96] AC 103 NNN> N=120 among (Nos 1-217)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAG2012]
[BAG2012]	(Bottacini+Ajello+Greiner, 2012)
Write:	<<[BAG2012] DDD.dddd+DD.ddddd>> <<[BAG2012] DDD.dddd+DD.dddd>> <<[BAG2012] DDD.dddd+DD.ddd>>
N:	113
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	N=113 sources from the Swift-INTEGRAL X-ray (SIX) survey, obtained by combining Swift/BAT and INTEGRAL/IBIS observations.
Ref:	=2012ApJS..201...34B
by	BOTTACINI E. , AJELLO M., GREINER J.
	Astrophys. J., Suppl. Ser., 201, 34 (2012)
	The deep look at the hard X-ray sky: the Swift-INTEGRAL X-ray (SIX) survey.
o	Table 2: <[BAG2012] DDD.dddd+DD.ddddd>, <[BAG2012] DDD.dddd+DD.dddd>, <[BAG2012] DDD.dddd+DD.ddd>, N=113.
=E=	Catalogue in electronic form as <J/ApJS/201/34/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAH2001]
[BAH2001]	(Brandt+Alexander+Hornschemeier+, 2001)
Write:	<<[BAH2001] NNN>> <<[BAH2001] SNN>>
N:	370+11
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS observations of the HDFN. N=370 sources and N=11 supplementary. See also CXOHDFN.
Ref:	=2001AJ....122.2810B
by	BRANDT W.N. , ALEXANDER D.M., HORNSCHEMEIER A.E., GARMIRE G.P., SCHNEIDER D.P., BARGER A.J., BAUER F.E., BROOS P.S., COWIE L.L., TOWNSLEY L.K., BURROWS D.N., CHARTAS G., FEIGELSON E.D., GRIFFITHS R.E., NOUSEK J.A., SARGENT W.L.W.
	Astron. J., 122, 2810-2832 (2001)
	The Chandra Deep Field North survey. V. 1 Ms source catalogs.
o	p.2831 (end of. ch.3.3): F36397+1547 = [DSB2001] F36397-1547, F36421+1545 = [HPA2000] J123642.16+621545.2.
o	Table 3: <[BAH2001] NNN> (Nos 1-370) = <CXOHDFN JHHMMSS.s+DDMMSS> N=370. Table 6: <[BAH2001] SNN> (Nos S1-S11) = <CXOHDFN JHHMMSS.s+DDMMSS> N=11.
=E=	Catalogue in electronic form as J/AJ/122/2810
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAH99]
[BAH99]	(Barvainis+Antonucci+Helou, 1999)
Write:	<<[BAH99] ACO 2219 N>>
N:	5
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	ISOCAM observations. Map in Fig.4
in source:	ACO 2219
Ref:	=1999AJ....118..645B
by	BARVAINIS R. , ANTONUCCI R., HELOU G.
	Astron. J., 118, 645-653 (1999)
	ISOCAM 15 micron search for distant infrared galaxies lensed by clusters.
o	T.1: G in ACO 2218 = LPS NNN.
o	Table 1: <[BAH99] ACO 2219 N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAK2008]
[BAK2008]	(Bilir+Ak+Karaali+, 2008)
Write:	<<[BAK2008] Pal5-SNNN>> <<[BAK2008] LNNN-SNNN>> <<[BAK2008] PGHHMM-SNNN>> <<[BAK2008] MNN-SNNNN>> <<[BAK2008] Draco-SNNN>> <<[BAK2008] Draco-Holtz-SNNN>> <<[BAK2008] NNNNN-SNNNN>> <<[BAK2008] LeoI-SNNNN>>
N:	773
Object:	* (SIMBAD class: Star)
Note:	Photometric catalog: all stars are 2MASS and SDSS objects.
Ref:	=2008MNRAS.384.1178B
by	BILIR S. , AK S., KARAALI S., CABRERA-LAVERS A., CHONIS T.S., GASKELL C.M.
	Mon. Not. R. Astron. Soc., 384, 1178-1188 (2008)
	Transformations between 2MASS, SDSS and BVRI photometric systems: bridging the near-infrared and optical.
o	Table 1: Objects LNNN = SA NNN in SIMBAD.
o	Table 1: <[BAK2008] Pal5-SNNN>, <[BAK2008] LNNN-SNNN>, <[BAK2008] PG HHMM-SNNN>, <[BAK2008] MNN-SNNNN>, <[BAK2008] Draco-SNNN>, <[BAK2008] Draco-Holtz-SNNN>, <[BAK2008] ANNNN-SNNNN>, <[BAK2008] LeoI-SNNNN>, N=773. Table 1: <Cl* NGC 2419 BAK DNN> N=4 among (Nos D4-D24), <Cl* NGC 4147 BAK DNN> N=5 among (Nos D3-D16).
=E=	Catalogue in electronic form as J/MNRAS/384/1178
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAL2007]
[BAL2007]	(Bergond+Athanassoula+Leon+, 2007)
Write:	<<[BAL2007] gcNNN.Na>> <<[BAL2007] gcNNN.NN>> <<[BAL2007] gcNNN.NNN>> <<[BAL2007] gcNNNNww>> <<[BAL2007] ucNNN.N>> <<[BAL2007] ucNNN.NN>> <<[BAL2007] ucdA>> <<[BAL2007] newdwN>>
N:	149+8+4
Object:	Poss. GlCl + UCO + G in ClG (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Stat:	is completely incorporated in Simbad
Note:	VLT FLAMES observations of the Fornax cluster.
in source:	NAME Fornax Cluster
Ref:	=2007A&A...464L..21B
by	BERGOND G. , ATHANASSOULA E., LEON S., BALKOWSKI C., CAYATTE V., CHEMIN L., GUZMAN R., MEYLAN G., PRUGNIEL P.
	Astron. Astrophys., 464L, 21-24 (2007)
	Globular clusters and dwarf galaxies in Fornax. I. Kinematics in the cluster core from multi-object spectroscopy.
o	In table 1 there are 2 objects designated as gc172.2, so we have added in the format a letter a and b to differentiate them.
o	Table 1: <[BAL2007] gcNNN.NNNa>, <[BAL2007] gcNNNNww>, N=149. Table 2: <[BAL2007] ucNNN.NN>, N=6, <[BAL2007] ucdA> (Nos A-B). Table 3: <[BAL2007] newdwN> (Nos 1-4).
=E=	Catalogue in electronic form as J/A+A/464/L21
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Baldone
Baldone	(Baldone obs.)
*****	Avoid the usage of Baldone, prefer BC
Details on Acronym: Balloon
Balloon	(Balloon number)= (BA)
Write:	<<Balloon FFFFFFNNN>>
N:	28+306
Object:	UV Exc. Obj. (SIMBAD class: UV = UV-emission Source)
Note:	SCAP exp. In the format, the first two FF stands for the flight number, the 4 last FFFF indicates up to 2 frames on which the star is seen, NNN is a running number.
Ref:	=1985A&AS...60..459T
by	TOBIN W.
	Astron. Astrophys., Suppl. Ser., 60, 459-470 (1985)
	Four-colour and H-β photometry of blue stars selected from a balloon-ultraviolet survey and other sources.
o	Table III: <Balloon FFffffNNN> N=28
Ref:	=1991A&A...250..370B
by	BIXLER J.V. , BOWYER S., LAGET M.
	Astron. Astrophys., 250, 370-388 (1991)
	A high galactic latitude survey of far-ultraviolet excess objects.
o	<Balloon FFffffNNN> N=306
=E=	Catalogue in electronic form as J/A+A/250/370
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BAM2001]
[BAM2001]	(Balaian+Akopian+Mikaelian+, 2001)
Write:	<<[BAM2001] IRAS HHMMm+DDMMa>>
N:	19
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=19 galaxies, possible counterpart of IRAS PSC sources.
Ref:	=2001AstL...27..284B
by	BALAIAN S.K. , AKOPIAN S.A., MIKAELIAN A.M., BURENKOV A.N.
	Astron. Lett., 27, 284-291 (2001)
	Optical studies of extragalactic infrared sources.
o	Table 1 : [BAM2001] IRAS 17442+6130 is a misprint for 6130b.
o	Table 1: <[BAM2001] IRAS HHMMm+DDMMa> N=19.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAM2019]
[BAM2019]	(Beuther+Ahmadi+Mottram+, 2019)
Write:	<<[BAM2019] mmNN>>
N:	12
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA cycle 3 1.3mm observations of N=12 millimeter sources in the star-forming region GAL 351.78-00.54.
in source:	GAL 351.78-00.54 = IRAS 17233-3606
Ref:	=2019A&A...621A.122B
by	BEUTHER H. , AHMADI A., MOTTRAM J.C., LINZ H., MAUD L.T., HENNING T., KUIPER R., WALSH A.J., JOHNSTON K.G., LONGMORE S.N.
	Astron. Astrophys., 621A, 122-122 (2019)
	High-mass star formation at sub-50 au scales.
o	Table 1: <[BAM2019] mmNN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAM98]
[BAM98]	(Bransford+Appleton+Marston+, 1998) (Not yet in Simbad)
Write:	<<[BAM98] LT 41 Knot N>> <<[BAM98] NGC 985 Knot N>> <<[BAM98] Arp 10 Knot N>> <<[BAM98] II Zw 28 Knot N>> <<[BAM98] II Hz 4 Knot N>> <<[BAM98] WN 1 Knot N>> <<[BAM98] VII Zw 466 Knot NN>> <<[BAM98] Abell 76 Knot N>>
N:	31
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
in source:	LT 41
in source:	NGC 985
in source:	APG 10
in source:	ZW II 28
in source:	NAME HZ II 4
in source:	NAME Sextans Ring
in source:	PN A66 76
Ref:	=1998AJ....116.2757B
by	BRANSFORD M.A. , APPLETON P.N., MARSTON A.P., CHARMANDARIS V.
	Astron. J., 116, 2757-2775 (1998)
	Multiwavelength observations of collisional ring galaxies. III. Oxygen/nitrogen abundances and star formation properties of ring knots.
o	Galaxy Abell 76 = PN A66 76, WN 1 = NAME SEXTANS RING
o	Table 5: <[BAM98] LT 41 Knot N> (Nos 1-3), <[BAM98] NGC 985 Knot N> (Nos 1-2), <[BAM98] Arp 10 Knot N> (Nos 1-6), <[BAM98] II Zw 28 Knot N> (No. 1), <[BAM98] II Hz 4 Knot N> (Nos 1-3), <[BAM98] WN 1 Knot N> (Nos 1-3), <[BAM98] VII Zw 466 Knot NN> (Nos 1-10), <[BAM98] Abell 76 Knot N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Bania
Bania	(Bania)
Write:	<<Bania Clump N>> <<Bania Arm>> <<Bania Clump 1 A>>
N:	4+1+8
Object:	MCld (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	1st ref., table 2: Clumps 1 and 2 and 3kpc Arm 2nd ref.: Clumps 3 and 4 are added. Table 4: format 'Clump 1 A', N=8 clouds in Clump 1
Ref:	=1977ApJ...216..381B
by	BANIA T.M.
	Astrophys. J., 216, 381-403 (1977)
	Carbon monoxide in the inner galaxy.
o	<Bania Clump N> N=2, <Bania Arm>
Ref:	=1986ApJ...307..350B
by	BANIA T.M. , STARK A.A., HEILIGMAN G.M.
	Astrophys. J., 307, 350-366 (1986)
	Clump 1: an unusual molecular cloud complex near the Galactic Center.
o	<Bania Clump N> (Nos 3-4) added. <Bania Clump 1 A> (Nos A-H)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BAO
BAO	(Beijing Astron. Obs.)
*****	Avoid the usage of BAO, prefer [EQL98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BAP2002]
[BAP2002]	(Bergeron+Aracil+Petitjean+, 2002)
Write:	<<[BAP2002] QSO J0331-3824 abs N.NNNN>> <<[BAP2002] QSO J0331-3824 abs N.NNNNN>>
N:	10+5
Object:	Absorber
Note:	VLT UVES spectrograph observations of QSO 0329-385 = QSO J0331-3824. 10 absorption systems are observed in the spectra and 5 sub-systems.
Ref:	=2002A&A...396L..11B
by	BERGERON J. , ARACIL B., PETITJEAN P., PICHON C.
	Astron. Astrophys., 396, 11-15 (2002)
	The warm-hot intergalactic medium at z~2.2: Metal enrichment and ionization source.
o	Table 1: <[BAP2002] QSO J0331-3824 abs N.NNNN> N=10. Table 2: <[BAP2002] QSO J0331-3824 abs N.NNNNN> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAR2014]
[BAR2014]	(Bayliss+Ashby+Ruel+, 2014)
Write:	<<[BAR2014] JHHMMSS.s+DDMMSS.s>>
N:	15 (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Magellan 6.5m Baade telescope IMACS optical spectroscopy of N=15 cluster member galaxies of the SPT-CL J2040-4451 galaxy cluster.
in source:	SPT-CL J2040-4451
Ref:	=2014ApJ...794...12B
by	BAYLISS M.B. , ASHBY M.L.N., RUEL J., BRODWIN M., AIRD K.A., BAUTZ M.W., BENSON B.A., BLEEM L.E., BOCQUET S., CARLSTROM J.E., CHANG C.L., CHO H.M., CLOCCHIATTI A., CRAWFORD T.M., CRITES A.T., DESAI S., DOBBS M.A., DUDLEY J.P., FOLEY R.J., FORMAN W.R., GEORGE E.M., GETTINGS D., GLADDERS M.D., GONZALEZ A.H., DE HAAN T., HALVERSON N.W., HIGH F.W., HOLDER G.P., HOLZAPFEL W.L., HOOVER S., HRUBES J.D., JONES C., JOY M., KEISLER R., KNOX L., LEE A.T., LEITCH E.M., LIU J., LUEKER M., LUONG-VAN D., MANTZ A., MARRONE D.P., MAWATARI K., McDONALD M., McMAHON J.J., MEHL J., MEYER S.S., MILLER E.D., MOCANU L., MOHR J.J., MONTROY T.E., MURRAY S.S., PADIN S., PLAGGE T., PRYKE C., REICHARDT C.L., REST A., RUHL J.E., SALIWANCHIK B.R., SARO A., SAYRE J.T., SCHAFFER K.K., SHIROKOFF E., SONG J., STALDER B., SUHADA R., SPIELER H.G., STANFORD S.A., STANISZEWSKI Z., STARK A.A., STORY K., STUBBS C.W., VAN ENGELEN A., VANDERLINDE K., VIEIRA J.D., VIKHLININ A., WILLIAMSON R., ZAHN O., ZENTENO A.
	Astrophys. J., 794, 12 (2014)
	SPT-CL J2040-4451: an SZ-selected galaxy cluster at z = 1.478 with significant ongoing star formation.
o	Table 2: <[BAR2014] JHHMMSS.s+DDMMSS.s> N=15.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Barbieri
Barbieri	(Barbieri+Bertola+Di tullio, 1974)
*****	Avoid the usage of Barbieri, prefer [BBD74]
Origin	of the Acronym: L (2004AN....325..307N)
Details on Acronym: Barhatova
Barhatova	(Barkhatova)= (Barkhatova)
Write:	<<Cl Barhatova N>>
N:	2
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Stat:	is completely incorporated in Simbad
Ref:	=1958SvA.....2..410B
by	BARKHATOVA K.A.
	Sov. Astron., 2, 410-419 (1958)
	Clusters in the region of the North America Nebula.
o	<Cl Barhatova N> (Nos 1-2)
Details on Acronym: Barkhatova
Barkhatova	(Barkhatova)
*****	Avoid the usage of Barkhatova, prefer Barhatova
Details on Acronym: Barn
Barn	(Barnard)
====>	Equivalent to: Barnard
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Barnard
Barnard	(Barnard)= (B) = Barn
Write:	<<Barnard NNNA>>
N:	370
Object:	Dark Cloud (SIMBAD class: DarkNeb = Dark Cloud (nebula))
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-370), but some numbering 'NNNA' (or 'NNNa' in literature) are inserted in RA.
Ref:	=1919ApJ....49....1B
by	BARNARD E.E.
	Astrophys. J., 49, 1-24 (1919)
	On the dark markings of the sky, with a catalogue of 182 such objects.
o	(Erratum) + erratum vol. 49, p. 360
o	Catalogue: <Barnard NNNA> (Nos 1-175), N=182.
Ref:	=1927Barn..C......0B
by	BARNARD E.E.
	Carnegie Inst. Washington D.C. Publ.,1927, 0-None (1927)
	A photographic Atlas of selected regions of the Milky Way.
o	<Barnard NNNA> N=349 among (Nos 1-370).
Ref:	=1988ApJ...324..311H
by	HEYER M.H.
	Astrophys. J., 324, 311-320 (1988)
	The magnetic evolution of the Taurus molecular clouds. II. A reduced role of the magnetic field in dense core regions.
o	(Erratum) + erratum vol. 329, 1039
o	Table 2: <HCl 2A> (Nos 2A-2F), <HCl 2GN> Nos 2G1, 2G2, <Barnard NNNA> (Nos 217A-217G) and (Nos 18A-18I)
Ref:	=2013MNRAS.432.1424K
by	KIRK J.M. , WARD-THOMPSON D., PALMEIRIM P., ANDRE Ph., GRIFFIN M.J., HARGRAVE P.J., KONYVES V., BERNARD J.-P., NUTTER D.J., SIBTHORPE B., DI FRANCESCO J., ABERGEL A., ARZOUMANIAN D., BENEDETTINI M., BONTEMPS S., ELIA D., HENNEMANN M., HILL T., MEN'SHCHIKOV A., MOTTE F., NGUYEN-LUONG Q., PERETTO N., PEZZUTO S., RYGL K.L.J., SADAVOY S.I., SCHISANO E., SCHNEIDER N., TESTI L., WHITE G.
	Mon. Not. R. Astron. Soc., 432, 1424-1433 (2013)
	First results from the Herschel Gould Belt survey in Taurus.
o	<Barnard NNNA> (No. 18J) added. Figs 5: <[KWP2013] NNN> (Nos 1-115).
=E=	Catalogue in electronic form as VII/220
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Barta
Barta	(Bartasiute)
Write:	<<Barta FFF NN>>
N:	78+54+79+70
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	ref. 1984VilOB..68...33B: field No. 112, format '112 NN', (Nos 1-78) ref. 1994BaltA...3..321B, Tables 1,2,3 col.(1): fields Nos 159, 161, 205, formats '159 NN' (Nos 1-54), '161 NN' (Nos 1-79), '205 NN' (Nos 1-70)
Ref:	=1984VilOB..68...33B
by	BARTASIUTE S.
	Vilnius Astron. Obs. Biul., 68, 33-41 (1984)
	Photoelectric photometry of stars near the North Galactic Pole in the Vilnius system. Kiev area 112.
o	Table 2, col.(1): <Barta 112 NN> (Nos 1-78)
Ref:	=1994BaltA...3..321B
by	BARTASIUTE S.
	Baltic Astronomy, 3, 321-334 (1994)
	Photoelectric Vilnius photometry of stars in the MEGA proper motion fields 159, 161 and 205 near the South Galactic Pole. I. Catalog of observations.
o	note in table 1 is erroneous read No 28 instead of 27
o	Table 1, col.(1): <Barta 159 NN> (Nos 1-54), col.KA: <Kiev 159 NNN> N=54 among (Nos 4-124). Table 2, col.(1): <Barta 161 NN> (Nos 1-79), col.KA: <Kiev 161 NNN> N=79 among (Nos 1-219). Table 3, col.(1): <Barta 205 NN> (Nos 1-70), col.KA: <Kiev 205 NNN> N=70 among (Nos 2-165)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BAS
BAS	(Bahcall+Soneira)
*****	Avoid the usage of BAS, prefer BSCG
Origin	of the Acronym: L (1997AJ....114.1297H)
Details on Acronym: [BAS98]
[BAS98]	(Brinchmann+Abraham+Schade+, 1998)= (CFRS) = (LDSS)
Write:	<<[BAS98] HH.NNNN>> <<[BAS98] HH.NNNNN>>
N:	341
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations. N=341 galaxies coming from the CFRS and LDSS surveys. In the format 'HH' stands for the field R.A. 'NNNN' always 4 digits when coming from the CFRS survey, 'NNNNN' always 5 digits when coming from the LDSS survey. See also CFRS, [GEC95], LDSS and LDSS-2.
Ref:	=1998ApJ...499..112B
by	BRINCHMANN J. , ABRAHAM R., SCHADE D., TRESSE L., ELLIS R.S., LILLY S., LE FEVRE O., GLAZEBROOK K., HAMMER F., COLLESS M., CRAMPTON D., BROADHURST T.
	Astrophys. J., 499, 112-133 (1998)
	Hubble space telescope imaging of the CFRS and LDSS redshift surveys. I. Morphological properties.
o	Table 2: <[BAS98] HH.NNNN>, <[BAS98] HH.NNNNN>, N=341.
=E=	Catalogue in electronic form as J/ApJ/499/112
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Basel
Basel	(Basel astr. institute)= (Basle) = (BF76)
Write:	<<Basel SA NNN-NNNNa>> <<Basel SA NNNF-NNNN>>
Object:	* (SIMBAD class: Star)
Note:	From the 9 vol. of 'Photometric catalogue for stars in selected areas and other fields in the RGU-system,' Becker + Fenkart, Astron. Institute of Basle. Only stars in Selected Areas in the RGU-system are in SIMBAD with the acronym 'Basel', for: * in SA 51, 54, 57, 71, 82, 94, 107, 133, 133F, 138, 141, 158
Auth.:	BECKER W.+
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Basel
Basel	(Basel astr. institute)= (Ba)
Write:	<<Cl Basel NNA>>
N:	20
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Note:	Cluster 11 is divided into 2 clusters A and B The last discovered cluster is Basel 20 = C 0931-561, Topaktas+ 1982, A&AS 49, 475-482
Ref:	=1965ZA.....60..249G
by	GRUBISSICH C.
	Zeitschr. Astrophys., 60, 249-255 (1965)
	Dreifarben-Photometrie von zwei offenen Sternhaufen in Richtung der Scutum-Wolke.
o	<Cl Basel 1>. Table 1: <Cl* NGC 6704 G NN> (Nos 1-52). Table 2: <Cl* Basel 1 G NN> (Nos 1-57).
Ref:	=1965ZA.....60..256G
by	GRUBISSICH C.
	Zeitschr. Astrophys., 60, 256-263 (1965)
	Dreifarben-Photometrie von zwei offenen Sternhaufen nahe NGC 7510.
o	CL Basel 2 = CL King 19, CL Basel 3 = CL Mrk 50 = CL Biurakan 3
o	<Cl Basel N> (Nos 2-3). Table 1: <Cl* King 19 G NN> (Nos 1-52). Table 2: <Cl Basel 3 NN> (Nos 1-60).
Ref:	=1965ZA.....61...97S
by	SVOLOPOULOS S.N.
	Zeitschr. Astrophys., 61, 97-104 (1965)
	The two distant open clusters King 8 and An. Basel 4.
o	<Cl Basel 4>
Details on Acronym: Basle
Basle	(Basel astr. institute)
*****	Avoid the usage of Basle, prefer Basel
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BASV
BASV	(Baade+Swope, Variable *)= (Baade Swope)
Write:	<<BASV NNN>>
N:	208
Object:	Exgl V* (SIMBAD class: Variable* = Variable Star)
Note:	See also other stars in Draco Dwarf Galaxy: [BS61]. See also [KHS2008], variable stars in Draco dwarf revisited..
in source:	NAME Draco Dwarf Galaxy
Ref:	=1961AJ.....66..300B
by	BAADE W. , SWOPE H.H.
	Astron. J., 66, 300-347 (1961)
	The Draco system, a dwarf galaxy.
o	Tables IV, V, VI, A, B, Plate III: <BASV NNN> (Nos 1-203). Table II: <[BS61] A> (Nos A-Z, No. I missing), <[BS61] AN> (Nos C1-C2, Q1-Q2), <[BS61] aaa> (Nos alf, bet, gam). Table C, Plate IV: <[BS61] NNNa> (Nos 1-595, 161a, 162a, 357a).
Ref:	=1976ApJ...209..734Z
by	ZINN R. , SEARLE L.
	Astrophys. J., 209, 734-747 (1976)
	The masses of the anomalous Cepheids in the Draco system.
o	<BASV NNN> (No. 204) added.
Ref:	=2002AJ....124.1464P
by	PRITZL B.J. , ARMANDROFF T.E., JACOBY G.H., DA COSTA G.S.
	Astron. J., 124, 1464-1485 (2002)
	The dwarf spheroidal companions to M31: variable stars in Andromeda VI.
o	Table 4: Ce* V1,V27,V51,V203 in Leo II are Swope VNNN, Ce* in Fornax: Author Pritzl writes to SIMBAD: objects objects 'FBW JHHMMSS.s+DDMMSS' are truncated to the last 3 digits, which would be the MSS at the end of their IDs.
o	Table 1: <[PAJ2002] VNNN> (Nos V1-V118). Table 4: <BASV NNN> (No. 208) added.
Details on Acronym: BASW
BASW	(Baade+Swope)= (H) = ([H29]) = (Hubble)
Write:	<<BASW NNN>> <<BASW NNN>>
N:	7+416
Object:	V* + Nova (SIMBAD class: Variable* = Variable Star)
Note:	Identif. charts. Field I in M 31. The numbering 'NNN' continues [H29] (Hubble 1929ApJ....69..103H) All V* among (Nos 1-467) have a idenditification 'BASW NNN' in SIMBAD. Field II and IV in M 31: see Gapo and [BS63]
in source:	M 31 = NGC 224
Ref:	=1929ApJ....69..103H
by	HUBBLE E.
	Astrophys. J., 69, 103-157 (1929)
	A spiral nebula as a stellar system, Messier 31.
o	Tables I, II, III: [H29] VNN use <BASW NN> (Nos 1-50). Tables IV, V: <[H29] ANN> N=63 among (Nos N1-N86).
Ref:	=1965AJ.....70..212B
by	BAADE W. , SWOPE H.H.
	Astron. J., 70, 212-268 (1965)
	Variables in the Andromeda galaxy - Fields I and III.
o	The numbering NNN continues the numbering of Hubble, 1929ApJ....69..103H. All V* among (Nos 1-467) have a idenditification 'BASW NNN' in SIMBAD.
o	Tables IV, VII, VIII: <BASW NNN> N=446 among (Nos 1-467). Table IV: <BASW AN> (Nos N1-N7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAT2008]
[BAT2008]	(Bradac+Allen+Treu+, 2008)
Write:	<<[BAT2008] BCGN>> <<[BAT2008] A D.dddddd+DD.ddddd>>
N:	3+11
Object:	G + Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations of MCS J0025.4-1222 field: N=3 Bright Cluster Galaxies (BCG) and N=4 multiply image systems (Nos A-D), with sub-images.
Ref:	=2008ApJ...687..959B
by	BRADAC M. , ALLEN S.W., TREU T., EBELING H., MASSEY R., MORRIS R.G., VON DER LINDEN A., APPLEGATE D.
	Astrophys. J., 687, 959-967 (2008)
	Revealing the properties of dark matter in the merging cluster MACS J0025.4-1222.
o	Fig.2, Table 1: <[BAT2008] BCGN> (Nos BCG1 to BCG3), <[BAT2008] A D.dddddd+DD.ddddd> N=11.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAT97]
[BAT97]	(Breysacher+Azzopardi+Testor+, 1997)
Write:	<<[BAT97] R>> <<[BAT97] R N>>
N:	5+12
Object:	Assoc. + * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=5 associations of NGC 300 surveyed for WR stars, (Nos I-V) Table 2, col(2): stars in each association
in source:	NGC 300
Ref:	=1997A&A...326..976B
by	BREYSACHER J. , AZZOPARDI M., TESTOR G., MURATORIO G.
	Astron. Astrophys., 326, 976-981 (1997)
	Wolf-Rayet stars detected in five associations of NGC 300.
o	Table 1: <[BAT97] R> (Nos I-V). Table 2, col(2): <[BAT97] I N> (Nos 1-2), <[BAT97] II N> (Nos 1-2), <[BAT97] III N> (No. 1), <[BAT97] IV N> (Nos 1-3), <[BAT97] V N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BAT99
BAT99	(Breysacher+Azzopardi+Testor+, 1999)= (LMC-WR)
Write:	<<BAT99 NNN>>
N:	134
Object:	WR (SIMBAD class: WolfRayet* = Wolf-Rayet)
Stat:	is completely incorporated in Simbad
Note:	Catalogue of all known Wolf-Rayet stars in the LMC
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1999A&AS..137..117B
by	BREYSACHER J. , AZZOPARDI M., TESTOR G.
	Astron. Astrophys., Suppl. Ser., 137, 117-145 (1999)
	The fourth catalogue of Population I Wolf-Rayet stars in the Large Magellanic Cloud.
o	Table 2: <BAT99 NNN> (Nos 1-134).
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: BAT99
BAT99	(Howarth+Walborn, 2012)
*****	Avoid the usage of BAT99, prefer [HW2012]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BATSE
BATSE	(1st BATSE catalog)
**	catalog: use 1B
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BATSE
BATSE	(2nd BATSE catalog)
**	catalog: use 2B
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BATSE
BATSE	(3rd BATSE catalog)
**	catalog: use 3B
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BATSE
BATSE	(4th BATSE catalog)
**	catalog: use 4B
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BATSE
BATSE	(BATSE catalog)
**	catalog: use BSAS
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BATSE
BATSE	(BATSE experiment)
*****	Avoid the usage of BATSE, prefer Trigger
Origin	of the Acronym: L (1997ApJS..110..157L)
Details on Acronym: Batten
Batten	(Batten)
*****	Avoid the usage of Batten, prefer SBC7
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Batten
Batten	(Batten+)
*****	Avoid the usage of Batten, prefer SBC8
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Baud
Baud	(Baud+)
*****	Avoid the usage of Baud, prefer BYB
Origin	of the Acronym: L (1998A&A...338..977C)
Details on Acronym: [BAW95]
[BAW95]	(Bontemps+Andre+Ward-Thompson, 1995)= (VLA)
Write:	<<[BAW95] N>>
N:	6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Also in Bontemps Thesis: [B96] LBS23 N. See also [AVE98].
in source:	NAME HH 24-26
Ref:	=1995A&A...297...98B
by	BONTEMPS S. , ANDRE P., WARD-THOMPSON D.
	Astron. Astrophys., 297, 98-102 (1995)
	Deep VLA search for the youngest protostars: a Class 0 source in the HH 24-26 region.
o	HH 24MMS = NAME HH 24MMS
o	<[BAW95] N> (Nos 1-6), <NAME HH 25MMS>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BAX
BAX	(Base de Donnees Amas de Galaxies X)
Write:	<<BAX DDD.dddd+DD.dddd>>
N:	1713
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	Multiwavelength database dedicated to X-ray clusters and groups of galaxies: http://bax.ast.obs-mip.fr
Ref:	=2004A&A...424.1097S
by	SADAT R. , BLANCHARD A., KNEIB J.-P., MATHEZ G., MADORE B., MAZZARELLA J.M.
	Astron. Astrophys., 424, 1097-1100 (2004)
	Introducing BAX: A database for X-ray clusters and groups of galaxies.
o	bax.dat: <BAX DDD.dddd+DD.dddd> N=1713.
=E=	Catalogue in electronic form as B/bax
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BAZ94]
[BAZ94]	(Bi+Arp+Zimmermann, 1994)
Write:	<<[BAZ94] NN>>
N:	46
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
in source:	NGC 3077
Ref:	=1994A&A...282..386B
by	BI H.G. , ARP H., ZIMMERMANN H.U.
	Astron. Astrophys., 282, 386-400 (1994)
	X-ray observations of NGC 3077.
o	<[BAZ94] NN> N=46
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BAZ97]
[BAZ97]	(Bridges+Ashman+Zepf+, 1997)
Write:	<<[BAZ97] 1-NN>> <<[BAZ97] 2-NN>>
N:	44+32
Object:	GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	Table 3a: GlCl candidates in M 104, format '1-NN' Table 3b: GlCl in field 2, format '2-NN'
in source:	M 104 = NGC 4594 = Sombrero Galaxy
Ref:	=1997MNRAS.284..376B
by	BRIDGES T.J. , ASHMAN K.M., ZEPF S.E., CARTER D., HANES D.A., SHARPLES R.M., KAVELAARS J.J.
	Mon. Not. R. Astron. Soc., 284, 376-384 (1997)
	Kinematics and metallicities of globular clusters in M104.
o	Table 3a: <[BAZ97] 1-NN> (Nos 1-1 to 1-44). Table 3b: <[BAZ97] 2-NN> (Nos 2-1 to 2-32)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BB
BB	(Barbieri+Benvenuti)
*****	Avoid the usage of BB, prefer A3
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BB
BB	(Bobylev+Bajkova)
*****	Avoid the usage of BB, prefer [BB2016]
Origin	of the Acronym: L (2016BaltA..25..377M)
Details on Acronym: BB
BB	(Brinks+Bajaja)
*****	Avoid the usage of BB, prefer [BB86]
Origin	of the Acronym: L (1988ARA&A..26..145T)
Details on Acronym: BB
BB	(Bok+Bok+)
*****	Avoid the usage of BB, prefer BBB
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BB
BB	(Boeshaar+Bond)
*****	Avoid the usage of BB, prefer BoBn
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BB
BB	(Batuski+Burns)
*****	Avoid the usage of BB, prefer SCC
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BB2000]
[BB2000]	(Braun+Burton, 2000)= ([BB2000a]) (Not yet in Simbad)
Write:	<<[BB2000] GLLL+BB+VVV A>>
N:	14
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Note:	Clumps 'A' in 6 HVC clouds.
in source:	NAME HVC G69+4-223
in source:	NAME HVC G115+13-275
in source:	NAME HVC G125+41-207
in source:	NAME HVC G204+30+75
in source:	NAME HVC G191+60+93
in source:	NAME HVC G230+61+165
Ref:	=2000A&A...354..853B
by	BRAUN R. , BURTON W.B.
	Astron. Astrophys., 354, 853-873 (2000)
	High-resolution imaging of compact high-velocity clouds.
o	Figs: <[BB2000] GLLL+BB+VVV A> N=3+3+2+4+1+1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB2000a]
[BB2000a]	(Braun+Burton, 2000) (Not yet in Simbad)
*****	Avoid the usage of [BB2000a], prefer [BB2000]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB2000b]
[BB2000b]	(Bocchino+Bykov, 2000)
Write:	<<[BB2000b] A>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	BeppoSAX observations of Hard X-ray emission from IC 443 (from BeppoSAX public archive).. Sources A and B are strong sources, source C is a weak extended hard X-ray emission region. See also [BB2003].
in source:	IC 443
Ref:	=2000A&A...362L..29B
by	BOCCHINO F. , BYKOV A.M.
	Astron. Astrophys., 362, 29-32 (2000)
	Hard X-ray emission from IC 443: evidence for a shocked molecular clump?
o	Fig.1, Table 2: <[BB2000b] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB2003]
[BB2003]	(Bocchino+Bykov, 2003)
Write:	<<[BB2003] NN>>
N:	12
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton observations of hard X-ray emission from the field of IC 443. N=12 detected sources. Source 11 contains several sources, see [BBP2005]. See also [BB2000b].
in source:	IC 443
Ref:	=2003A&A...400..203B
by	BOCCHINO F. , BYKOV A.M.
	Astron. Astrophys., 400, 203-211 (2003)
	XMM-Newton study of hard X-ray sources in IC 443.
o	Table 2 : Src A, B = [BB2000b] A, B.
o	Table 2: <[BB2003] NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB2006]
[BB2006]	(Briggs+Barnes, 2006)= (WSRT)
Write:	<<[BB2006] JHHMMSS+DDMM>>
N:	2
Object:	HI Cloud (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	Westerbork Synthesis Radio Telescope observations of HI emitters in the field of PG 1216+069.
Ref:	=2006ApJ...640L.127B
by	BRIGGS F.H. , BARNES D.G.
	Astrophys. J., 640, 127-130 (2006)
	H I 21 cm observations of the PG 1216+069 sub-damped Lyα absorber field at z = 0.00632.
o	Table 2: WSRT 1216+064 and SDSS 1219+0616 not identified.
o	Text: <[BB2006] JHHMMSS+DDMM> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB2009]
[BB2009]	(Boudreault+Bailer-Jones, 2009)
Write:	<<[BB2009] IC2391-WFI-FF-NNN>>
N:	3111
Object:	* (SIMBAD class: Star)
Note:	ESO 2.2m WFI, CTIO CPAPIR, CTIO HYDRA observations of the open cluster IC 2391.
in source:	IC 2391
Ref:	=2009ApJ...706.1484B
by	BOUDREAULT S. , BAILER-JONES C.A.L.
	Astrophys. J., 706, 1484-1503 (2009)
	A constraint on brown dwarf formation via ejection: radial variation of the stellar and substellar mass function of the young open cluster IC 2391.
o	In table 3, some mix-up with "ID" numbers; refer to table 2 by coordinates or VizieR version for the correct IDs in table 3.
o	Table 2: <[BB2009] IC2391-WFI-FF-NNN> N=3111.
=E=	Catalogue in electronic form as <J/ApJ/706/1484/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB2010]
[BB2010]	(Burke-Spolaor+Bailes, 2010) (Not yet in Simbad)
Write:	<<[BB2010] JHHMM+DD>>
N:	14
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB2016]
[BB2016]	(Bobylev+Bajkova, 2016)= (BB)
Write:	<<[BB2016] NN>>
N:	24
Object:	Moving Group (SIMBAD class: MouvGroup = Moving Group)
Note:	N=24 moving groups in RAVE4 data.
Ref:	=2016AstL...42...90B
by	BOBYLEV V.V. , BAJKOVA A.T.
	AstL, 42, 90-99 (2016)
	Kinematic analysis of solar-neighborhood stars based on RAVE4 data.
o	2016PAZh...42..110B
o	Table 3: <[BB2016] NN> (Nos 1-24).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB69]
[BB69]	(Bok+Bok, 1969)
Write:	<<[BB69] LMC NN>> <<[BB69] GL Car NN>> <<[BB69] HD 101545 NN>> <<[BB69] IC 2944 NN>> <<[BB69] Cen N>> <<[BB69] Nor R NN>> <<[BB69] SA NNN NN>>
N:	114
Object:	* (SIMBAD class: Star)
Note:	Tables I to XI: photoelectric sequences in 11 fields
Ref:	=1969AJ.....74.1125B
by	BOK B.J. , BOK P.F.
	Astron. J., 74, 1125-1130 (1969)
	Photometric standards for the southern hemisphere.
o	Table I: <[BB69] LMC NN> (Nos 1-16). Table III: <[BB69] GL Car NN> (Nos 1-14). Table IV: <[BB69] HD 101545 NN> (Nos 1-19). Table V: <[BB69] IC 2944 NN> (Nos 1-12). Table VIII: <[BB69] Cen N> (Nos 1-7). Table IX: <[BB69] Nor I NN> (Nos 1-13), <[BB69] Nor II N> (Nos 1-5), <[BB69] Nor III N> (Nos 1-4). Table X: <[BB69] SA 169 NN> (Nos 1-10). Table XI: <[BB69] SA 205 NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB70]
[BB70]	(Bahcall+Bahcall, 1970)= (B	B)
Write:	<<[BB70] Ton 256 NN>> <<[BB70] B NNN NN>> <<[BB70] 3C 273 NN>> <<[BB70] PKS HHMM+DD NN>> <<[BB70] PHL 1093 NN>>
N:	42+88
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Galaxies in the direction of QSOs Identif. charts
Ref:	=1970PASP...82..721B
by	BAHCALL J.N. , BAHCALL N.A.
	Publ. Astron. Soc. Pac., 82, 721-729 (1970)
	On the galaxies in the direction of TON 256 and B 264.
o	B 264 = [B68b] 264
o	Table I: <[BB70] Ton 256 NN> (Nos 1-21). Table II: <[BB70] B 264 NN> (Nos 1-21).
Ref:	=1970PASP...82.1276B
by	BAHCALL N.A. , BAHCALL J.N.
	Publ. Astron. Soc. Pac., 82, 1276-1292 (1970)
	Galaxies in the direction of QSO's with small redshifts.
o	B 234, 340 = [B68b] 234 and [B68b] 340
o	Table I: <[BB70] 3C 273 NN> (Nos 1-15). Table II: <[BB70] B 234 NN> (Nos 1-15). Table III: <[BB70] B 340 NN> (Nos 1-12). Table IV: <[BB70] PKS 0736+01 NN> (Nos 1-11). Table V: <[BB70] PKS 0837-12 NN> (Nos 1-11). Table VI: <[BB70] PKS 2135-14 NN> (Nos 1-12). Table VII: <[BB70] PHL 1093 NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB74]
[BB74]	(Brandie+Bridle, 1974)= (MA) (Not yet in Simbad)
Write:	<<[BB74] HHMM+DD>>
N:	55
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ν = 8000MHz, HPBW = 5.9'
Ref:	=1974AJ.....79..903B
by	BRANDIE G.W. , BRIDLE A.H.
	Astron. J., 79, 903-917 (1974)
	Optical identifications and radio spectra of sources found by the Michigan 8-GHz survey.
o	Table II: <[BB74] HHMM+DD> N=55
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB84]
[BB84]	(Blanco+Blanco, 1984)
Write:	<<[BB84] NN>>
N:	70
Object:	* (SIMBAD class: Star)
Ref:	=1984PASP...96..603B
by	BLANCO V.M. , BLANCO B.M.
	Publ. Astron. Soc. Pac., 96, 603-608 (1984)
	A B, V sequence in Baade's Window.
o	cross-id: col.(2): Cl* NGC 6522 ARP A ou a, Cl* NGC 6522 VDB aaa (greek letter). col.(3): Cl* NGC 6522 ARP R-NNN
o	Table I: <[BB84] NN> (Nos 1-70)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB85]
[BB85]	(Batuski+Burns, 1985) (Not yet in Simbad)
Write:	<<[BB85] Void NN>>
N:	23
Object:	Void (SIMBAD class: Void = Underdense Region of the Universe)
Note:	Table III: N=23 nearby voids in the distribution of ACO clusters See also [EET94], [S2000h]. Table I: N=102 supercluster candidates SCC
Ref:	=1985AJ.....90.1413B
by	BATUSKI D.J. , BURNS J.O.
	Astron. J., 90, 1413-1424 (1985)
	Finding lists of candidate superclusters and voids of Abell clusters.
o	T.III: voids not in SIMBAD
o	Tables I(a), I(b): <SCC NNN> (Nos 1-102). Table III: <[BB85] Void NN> (Nos 1-23)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB86]
[BB86]	(Brinks+Bajaja, 1986)= (BB) = ([BB86a])
Write:	<<[BB86] NNN>>
N:	141
Object:	HI Hole (SIMBAD class: PartofG = Part of a Galaxy)
Note:	N=141 HI Holes in M 31
in source:	M 31 = NGC 224
Ref:	=1986A&A...169...14B
by	BRINKS E. , BAJAJA E.
	Astron. Astrophys., 169, 14-42 (1986)
	A high-resolution hydrogen-line survey of Messier 31. III. HI holes in the interstellar medium.
o	Table 2: <[BB86] NNN> (Nos 1-141)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB86a]
[BB86a]	(Brinks+Bajaja, 1986)
*****	Avoid the usage of [BB86a], prefer [BB86]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB86b]
[BB86b]	(Bergeron+Boisse, 1986)
Write:	<<[BB86b] PKS 1912-54 NN>> <<[BB86b] PKS 2135-14 NN>>
N:	17+13
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 4: N=17 objects in the field of the QSO 'PKS 1912-54' Table 5: N=13 objects in the field of the QSO 'PKS 2135-14' See also [B86b], [BDK87], [B88], [BBK88], [BB91], [BCS92], [GB97]
Ref:	=1986A&A...168....6B
by	BERGERON J. , BOISSE P.
	Astron. Astrophys., 168, 6-10 (1986)
	Nature of the Za - Ze absorption line systems in the QSOs PKS 1912-54 and PKS 2135-14.
o	Table 4: <[BB86b] PKS 1912-54 NN> (Nos 1-17). Table 5: <[BB86b] PKS 2135-14 NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB87]
[BB87]	(Buczilowski+Beck, 1987)
*****	Avoid the usage of [BB87], prefer [VBW78]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB90]
[BB90]	(Boisse+Boulade, 1990)
Write:	<<[BB90] NN>> <<[BB90] GN>>
N:	16
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Study of the field of 3C 196: N=16 objects (Nos 1-16), among which N=2 galaxies. G1 noticed in 1963ApJ...138...30M.
Ref:	=1990A&A...236..291B
by	BOISSE P. , BOULADE O.
	Astron. Astrophys., 236, 291-298 (1990)
	An optical study of the z = 0.437 21-cm absorber in front of 3C 196.
o	In reference list and text, Mathews should be Matthews.
o	Table 2: <[BB90] NN> (Nos 1-16), <[BB90] GN> (Nos G1-G2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB91]
[BB91]	(Bergeron+Boisse, 1991)
Write:	<<[BB91] HHMM+DDd GN>>
N:	60
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 2: N=60 objects in 10 QSO fields Among these objects 20 are in Table 4 as galaxies, sometimes found with the format 'GN' See also [B86b], [BB86b], [BDK87], [B88], [BBK88], [BCS92], [GB97]
Ref:	=1991A&A...243..344B
by	BERGERON J. , BOISSE P.
	Astron. Astrophys., 243, 344-366 (1991)
	A sample of galaxies giving rise to Mg II quasar absorption systems.
o	Table 2: <[BB91] HHMM+DDd GN> N=60
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB92]
[BB92]	(Beauchemin+Borra, 1992)
Write:	<<[BB92] HHMM+DDMMA>>
N:	32
Object:	Lensed Image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	Tables 2 and 4: rounded coordinates, N=16 lens pair candidates. Finding charts
Ref:	=1992AJ....103..405B
by	BEAUCHEMIN M. , BORRA E.F.
	Astron. J., 103, 405-412 (1992)
	An automated search for widely spaced gravitational lenses performed on 25 Grens plates.
o	Tables 2, 4: <[BB92] HHMM+DDMMA> N=32
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB93]
[BB93]	(Beauchemin+Borra, 1993)
Write:	<<[BB93] NN>>
N:	36
Object:	Stellar obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Finding charts
Ref:	=1993AJ....105.1587B
by	BEAUCHEMIN M. , BORRA E.F.
	Astron. J., 105, 1587-1595 (1993)
	Classification algorithms applied to 10588low-resolution slitless spectra: a search for unusual and interesting objects.
o	<[BB93] NN> N=36
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB96]
[BB96]	(Baudry+Brouillet, 1996)
Write:	<<[BB96] Region SN>> <<[BB96] HHMMSS.s+DDMMSS.s>> <<[BB96] HHMMSS.s+DDMMSS.ss>>
N:	4+7
Object:	Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	Table 3: N=4 H2O Maser regions, (Nos S1-S4) Table 4: N=7 possible H2O maser detections, format 'HHMMSS.s+DDMMSS.ss' or 'HHMMSS.s+DDMMSS.s'
in source:	M 82 = NGC 3034
Ref:	=1996A&A...316..188B
by	BAUDRY A. , BROUILLET N.
	Astron. Astrophys., 316, 188-195 (1996)
	Spatial distribution and nature of H_{2}O masers in Messier 82.
o	T.5: M1, 2 = [WFG84] m1, 2. p. 190: BBH Group R
o	Table 3: <[BB96] Region SN> (Nos S1-S4). Table 4: <[BB96] HHMMSS.s+DDMMSS.ss> or <[BB96] HHMMSS.s+DDMMSS.s> N=7
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB97]
[BB97]	(Brazier+Becker, 1997)= ([BB97a])
Write:	<<[BB97] NNN>>
N:	11
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations Table 1: Knots in the vicinity of RCW 89 Fig.2: Map
Ref:	=1997MNRAS.284..335B
by	BRAZIER K.T.S. , BECKER W.
	Mon. Not. R. Astron. Soc., 284, 335-340 (1997)
	High-resolution X-ray imaging of the supernova remnant MSH 15-52.
o	Table 1: <[BB97] ANN> (Nos N0-N10)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB97a]
[BB97a]	(Brazier+Becker, 1997)
*****	Avoid the usage of [BB97a], prefer [BB97]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB97c]
[BB97c]	(Blanco+Blanco, 1997)
Write:	<<[BB97c] NN>> <<[BB97c] EN>>
N:	63+3
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=63 RR Lyrae stars + N=3 eclipsing stars Fig.2: Identif. charts
in source:	NAME Galactic Bulge
Ref:	=1997AJ....114.2596B
by	BLANCO B.M. , BLANCO V.M.
	Astron. J., 114, 2596-2603 (1997)
	RR Lyrae variables in a new galactic bulge window.
o	Table 1: <[BB97c] NN> (Nos 1-63), <[BB97c] EN> (Nos E1-E3).
=E=	Catalogue in electronic form as J/AJ/114/2596
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BB99]
[BB99]	(Braun+Burton, 1999)
Write:	<<[BB99] NN>>
N:	66
Object:	HVC (SIMBAD class: HVCld = High-velocity Cloud)
Stat:	is completely incorporated in Simbad
Note:	See also [SB2002].
Ref:	=1999A&A...341..437B
by	BRAUN R. , BURTON W.B.
	Astron. Astrophys., 341, 437-450 (1999)
	The kinematic and spatial deployment of compact, isolated high-velocity clouds.
o	Table 1: <[BB99] NN> (Nos 1-66).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBA2004]
[BBA2004]	(Burbidge+Burbidge+Arp+, 2004) (Not yet in Simbad)
Write:	<<[BBA2004] NGC 2639 CN.NA>>
N:	4
Object:	QSO (SIMBAD class: QSO = Quasar)
Note:	ROSAT PSPC observations observations reveal four X-ray sources identified as QSOs associated with NGC 2639. The format 'CN.NA' stands for C1.4A, C2.0, C2.4 and C2.6 counts.ks(-1).
Ref:	=2004ApJS..153..159B
by	BURBIDGE E.M. , BURBIDGE G., ARP H.C., ZIBETTI S.
	Astrophys. J., Suppl. Ser., 153, 159-163 (2004)
	QSOs and active galactic nuclei associated with NGC 2639.
o	Table 1: <[BBA2004] NGC 2639 CN.NA> (Nos C1.4A, C2.0, C2.4, C2.6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBA2006]
[BBA2006]	(Brodwin+Brown+Ashby+, 2006)= (IRAC)
Write:	<<[BBA2006] IRAC JHHMMSS.s+DDMMSS>>
N:	8
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC Shallow Survey: discovery of a new cluster ClG J1434+3427, and 8 member galaxies. See also [ESB2004] and [SEB2005].
in source:	ClG J1434+3427
Ref:	=2006ApJ...651..791B
by	BRODWIN M. , BROWN M.J.I., ASHBY M.L.N., BIAN C., BRAND K., DEY A., EISENHARDT P.R., EISENSTEIN D.J., GONZALEZ A.H., HUANG J.-S., JANNUZI B.T., KOCHANEK C.S., McKENZIE E., MURRAY S.S., PAHRE M.A., SMITH H.A., SOIFER B.T., STANFORD S.A., STERN D., ELSTON R.J.
	Astrophys. J., 651, 791-803 (2006)
	Photometric redshifts in the IRAC shallow survey.
o	ISCS J1434.5+3427: Too short format for ISCS clusters, ClG J1434+3427 in SIMBAD.
o	Table 5: <[BBA2006] IRAC JHHMMSS.s+DDMMSS> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBA2008]
[BBA2008]	(Beirao+Brandl+Appleton+, 2008)
Write:	<<[BBA2008] Region N>>
N:	4 (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRS observations of M 82.
in source:	M 82
Ref:	=2008ApJ...676..304B
by	BEIRAO P. , BRANDL B.R., APPLETON P.N., GROVES B., ARMUS L., FORSTER SCHREIBER N.M., SMITH J.D., CHARMANDARIS V., HOUCK J.R.
	Astrophys. J., 676, 304-316 (2008)
	Spatially resolved Spitzer IRS spectroscopy of the central region of M82.
o	Table 1 : <[BBA2008] Region N> (Nos 1-4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBA2019]
[BBA2019]	(Bosco+Beuther+Ahmadi+, 2019) (Not yet in Simbad)
Write:	<<[BBA2019] IRAS 23033+5951-MMS1c>>
N:	1
Object:	Dense Core (SIMBAD class: denseCore = Dense Core)
Note:	NOEMA 1.37 mm observations of N=1 continuum source in IRAS 23033+5951.
in source:	IRAS 23033+5951
Ref:	=2019A&A...629A..10B
by	BOSCO F. , BEUTHER H., AHMADI A., MOTTRAM J.C., KUIPER R., LINZ H., MAUD L., WINTERS J.M., HENNING T., FENG S., PETERS T., SEMENOV D., KLAASSEN P.D., SCHILKE P., URQUHART J.S., BELTRAN M.T., LUMSDEN S.L., LEURINI S., MOSCADELLI L., CESARONI R., SANCHEZ-MONGE A., PALAU A., PUDRITZ R., WYROWSKI F., LONGMORE S.
	Astron. Astrophys., 629A, 10-10 (2019)
	Fragmentation, rotation, and outflows in the high-mass star-forming region IRAS 23033+5951. A case study of the IRAM NOEMA large program CORE.
o	Table 3: <[BBA2019] IRAS 23033+5951-MMS1c> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BBB
BBB	(Bok+Bok+Basinski)= (BB)
Write:	<<BBB LMC NN>> <<BBB SMC NNN>> <<BBB a>> <<BBB BN>>
N:	79+9+377+9
Object:	* (SIMBAD class: Star)
Note:	In LMC (1962MNRAS.123..487B): Tables I and V: format 'NN', (Nos 1-60), in the fields of NGC 1955 and NGC 1968-1974. (Nos 61-79) are only on Plate II(b). Table IV: format 'a', (Nos a-h, j), photoelectric standards. In SMC (1967MNRAS.137...55B): Table I, Plate 1: format 'BN', (Nos B1-B9), standards stars. Table V, Plate 2: (Nos 1-377).
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1962MNRAS.123..487B
by	BOK B.J. , BOK P.F., BASINSKI J.M.
	Mon. Not. R. Astron. Soc., 123, 487-496 (1962)
	Colour-magnitude arrays for two associations in the Large Magellanic Cloud.
o	Tables I, V, Plate II(b): <BBB LMC NN> (Nos 1-79). Tables III, IV: <BBB a> (Nos a-h, j).
Ref:	=1967MNRAS.137...55B
by	BASINSKI J.M. , BOK B.J., BOK P.F.
	Mon. Not. R. Astron. Soc., 137, 55-67 (1967)
	A colour-magnitude array for a region in the core of the Small Magellanic Cloud.
o	Table I: <BBB BN> (Nos B1-B9). Table V: <BBB SMC NNN> (Nos 1-377).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BBB2004]
[BBB2004]	(Bravo-Alfaro+Brunks+Baker+, 2004)= ([BBB2004a])
Write:	<<[BBB2004] HI A>> <<[BBB2004] CO WW>>
N:	3+2
Object:	HI Cloud + CO Cloud (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLA observations (letter 'A' in the format) and OSRO observations (letters 'WW' in the format) from IRAM observations. N=3 HI clouds, and N=2 CO concentrations in the galaxy Haro 2 (= [H56] 2 in SIMBAD). The CO concentrations were already described in Fritz Ph.D Thesis, 2000.
in source:	[H56] 2
Ref:	=2004AJ....127..264B
by	BRAVO-ALFARO H. , BRINKS E., BAKER A.J., WALTER F., KUNTH D.
	Astron. J., 127, 264-278 (2004)
	H I and CO in blue compact dwarf galaxies: Haro 2 and Haro 4.
o	Fig.3: <[BBB2004] HI A> (Nos A-C). Fig.5: <[BBB2004] CO WW> (Nos S, NW).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBB2004a]
[BBB2004a]	(Bravo-Alfaro+Brunks+Baker+, 2004)
*****	Avoid the usage of [BBB2004a], prefer [BBB2004]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBB2004b]
[BBB2004b]	(Bird+Barlow+Bassani+, 2004)
*****	Avoid the usage of [BBB2004b], prefer INTEGRAL1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBB2004c]
[BBB2004c]	(Barr+Baker+Bremer+, 2004)
Write:	<<[BBB2004c] BHHMM+DDd NN>>
N:	5+11+10+7+5+9
Object:	G (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Taurus Tunable Filter observations at the Anglo-Australian Telescope. Search for new Emission-Line Galaxies (ELG) in the field of 6 MRC QSOs.
Ref:	=2004AJ....128.2660B
by	BARR J.M. , BAKER J.C., BREMER M.N., HUNSTEAD R.W., BLAND-HAWTHORN J.
	Astron. J., 128, 2660-2676 (2004)
	Tunable-filter imaging of quasar fields at z ~ 1. II. The star-forming galaxy environments of radio-loud quasars.
o	Table 2: <[BBB2004c] BHHMM+DDd NN> N=5+11+10+7+5+9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBB73]
[BBB73]	(Barbier+Bernard+Bigay+, 1973)
Write:	<<[BBB73] NNN>>
N:	340
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	No. 195 is missing in table, but present in the chart, it corresponds to the second No. 329, who have not to exist.
Ref:	=1973A&A....27..421B
by	BARBIER M. , BERNARD A., BIGAY J.H., GARNIER R.
	Astron. Astrophys., 27, 421-427 (1973)
	Galactic structure in the direction of Cep.
o	Table 1: <[BBB73] NNN> (Nos 1-341, No. 317 missing).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBB99]
[BBB99]	(Benitez+Broadhurst+Bouwens+, 1999)
Write:	<<[BBB99] NIC3 ETN>> <<[BBB99] NIC3 SPN>>
N:	4+2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=6 galaxies in the HDF NIC3 field. In the format ET stands for Early Type, SP for Spheroidal Profile(?).
in source:	NAME HDFN
Ref:	=1999ApJ...515L..65B
by	BENITEZ N. , BROADHURST T., BOUWENS R., SILK J., ROSATI P.
	Astrophys. J., 515, 65-68 (1999)
	Detection of evolved high-redshift galaxies in deep NICMOS/VLT images.
o	Table 1, Fig.1: <[BBB99] NIC3 ETN> (Nos ET1-ET4), <[BBB99] NIC3 SPN> (Nos SP1-SP2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBC017]
[BBC017]	(Beuret+Billot+Cambresy+, 2017) (Not yet in Simbad)
Write:	<<[BBC017] GLLL.ll+BB.bbb>>
Object:	Poss. Cluster of * (SIMBAD class: Cluster*_Candidate = Cluster of Stars Candidate)
Note:	N=496+1137 cluster candidates and potential cluster candidates, found in the Herschel infrared Galactic Plane Survey (Hi-GAL).
Ref:	=2017A&A...597A.114B
by	BEURET M. , BILLOT N., CAMBRESY L., EDEN D.J., ELIA D., MOLINARI S., PEZZUTO S., SCHISANO E.
	Astron. Astrophys., 597A, 114-114 (2017)
	Source clustering in the Hi-GAL survey determined using a minimum spanning tree method.
o	Tables 1-2: <[BBC017] GLLL.ll+BB.bbb> N=496+1137.
=E=	Catalogue in electronic form as <J/A+A/597/A114/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBC2000]
[BBC2000]	(Buson+Bertola+Capellari+, 2000)
Write:	<<[BBC2000] NN>>
N:	60
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations. Map in Fig.1
in source:	ACO 851 = ClG 0939+4713
Ref:	=2000ApJ...531..684B
by	BUSON L.M. , BERTOLA F., CAPPELLARI M., CHIOSI C., DRESSLER A., OEMLER A.Jr
	Astrophys. J., 531, 684-692 (2000)
	Ultraviolet imaging of the galaxy cluster CL 0939+4713 (Abell 851) at z=0.41.
o	Table 1: <[BBC2000] NN> (Nos 1-60).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBC2003]
[BBC2003]	(Butt+Benaglia+Combi+, 2003)
Write:	<<[BBC2003] XS 04358.BN-NNN>>
N:	20
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of the field of the source TeV J2032+4131. These objects are later defined as 'ChaMP XS04358BN-NNN', see ChaMP.
Ref:	=2003ApJ...597..494B
by	BUTT Y.M. , BENAGLIA P., COMBI J.A., CORCORAN M., DAME T.M., DRAKE J., KAUFMAN BERNADO M.M., MILNE P., MINIATI F., POHL M., REIMER O., ROMERO G.E., RUPEN M.
	Astrophys. J., 597, 494-512 (2003)
	Chandra/Very Large Array follow-up of TeV J2032+4131, the only unidentified TeV γ-ray source.
o	The [BBC2003] objects are later found in literature as 'ChaMP XS04358BN-NNN'.
o	Tables 2, 3: <[BBC2003] XS 04358.BN-NNN> N=20.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBC2005]
[BBC2005]	(Broadhurst+Benitez+Coe+, 2005)
Write:	<<[BBC2005] NN.N>> <<[BBC2005] NN.Na>> <<[BBC2005] Source NN>>
N:	105+18+49+5
Object:	Arc (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	Advanced Camera Images on HST observations of ACO 1689. Multiple images (Arcs) of 30 sources (first digits NN in the format).
in source:	ACO 1689
Ref:	=2005ApJ...621...53B
by	BROADHURST T. , BENITEZ N., COE D., SHARON K., ZEKSER K., WHITE R., FORD H., BOUWENS R., BLAKESLEE J., CLAMPIN M., CROSS N., FRANX M., FRYE B., HARTIG G., ILLINGWORTH G., INFANTE L., MENANTEAU F., MEURER G., POSTMAN M., ARDILA D.R., BARTKO F., BROWN R.A., BURROWS C.J., CHENG E.S., FELDMAN P.D., GOLIMOWSKI D.A., GOTO T., GRONWALL C., HERRANZ D., HOLDEN B., HOMEIER N., KRIST J.E., LESSER M.P., MARTEL A.R., MILEY G.K., ROSATI P., SIRIANNI M., SPARKS W.B., STEINDLING S., TRAN H.D., TSVETANOV Z.I., ZHENG W.
	Astrophys. J., 621, 53-88 (2005)
	Strong-lensing analysis of A1689 from deep advanced camera images.
o	In subject headings A1683 is a misprint for A1689. MS 2137 = MS 2137.3-2353, clusters MS 0404 and MS 1417+22 not identified (MS 1417+22 not in ref. Gavazzi et al. 2003)
o	Table 2, Fig.4: <[BBC2005] NN.N> N=105 (Nos 1.1-1.6 to 30.1-30.3). Fig. 5-8: <[BBC2005] Source NN> (Nos 1-30).
Ref:	=2007ApJ...668..643L
by	LIMOUSIN M. , RICHARD J., JULLO E., KNEIB J.-P., FORT B., SOUCAIL G., ELIASDOTTIR A., NATARAJAN P., ELLIS R.S., SMAIL I., CZOSKE O., SMITH G.P., HUDELOT P., BARDEAU S., EBELING H., EGAMI E., KNUDSEN K.K.
	Astrophys. J., 668, 643-666 (2007)
	Combining strong and weak gravitational lensing in Abell 1689.
o	Fig.1, Table 1: <[BBC2005] NN.N> N=18 (Nos 31.1-31.4 to 40.1-40.2). Table 2: <[LRJ2007] Galaxy N> (Nos 1-5).
Ref:	=2015MNRAS.446..683D
by	DIEGO J.M. , BROADHURST T., BENITEZ N., UMETSU K., COE D., SENDRA I., SERENO M., IZZO L., COVONE G.
	Mon. Not. R. Astron. Soc., 446, 683-704 (2015)
	A free-form lensing grid solution for A1689 with new multiple images.
o	Table A1: <[BBC2005] NN.N> N=49 (Nos 41.1-41.3 to 61.1-61.3) added, <[BBC2005] NN.Na> N=5 (Nos 25.2a, 25.2b, 25.2c, 32.5a, 32.5b) added.
=E=	Catalogue in electronic form as J/ApJ/621/53
=E=	Catalogue in electronic form as J/ApJ/668/643
=E=	Catalogue in electronic form as <J/MNRAS/446/683/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBC2006]
[BBC2006]	(Beltran+Brand+Cesaroni+, 2006)
Write:	<<[BBC2006] IRAS HHMMm+DDMM Clump NN>>
N:	763
Object:	Clump (SIMBAD class: denseCore = Dense Core)
Note:	SEST SIMBA 1.2mm observations of dust clumps towards 227 IRAS PSC sources.
Ref:	=2006A&A...447..221B
by	BELTRAN M.T. , BRAND J., CESARONI R., FONTANI F., PEZZUTO S., TESTI L., MOLINARI S.
	Astron. Astrophys., 447, 221-233 (2006)
	Search for massive protostar candidates in the southern hemisphere. II. Dust continuum emission.
o	Table 2: <[BBC2006] IRAS HHMMm+DDMM Clump NN> N=763.
=E=	Catalogue in electronic form as J/A+A/447/221
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBC2012]
[BBC2012]	(Buzzoni+Bertone+Carraro+, 2012) (Not yet in Simbad)
Write:	<<[BBC2012] a>>
N:	3
Object:	* (SIMBAD class: Star)
Note:	TNG observations of N=3 stars in the field of NGC 6791.
in source:	NGC 6791
Ref:	=2012ApJ...749...35B
by	BUZZONI A. , BERTONE E., CARRARO G., BUSON L.
	Astrophys. J., 749, 35 (2012)
	Stellar lifetime and ultraviolet properties of the old metal-rich galactic open cluster NGC 6791: a pathway to understand the ultraviolet upturn of elliptical galaxies.
o	Figure 3: star "c" = [CBB2013b] 1812 in Simbad (cf 2013AJ....146..128C).
o	Fig. 3: <[BBC2012] a> (Nos a-c).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBC2018]
[BBC2018]	(Brocato+Branchesi+Cappellaro+, 2018)
Write:	<<[BBC2018] VSTJDDD.ddddd+DD.ddddd>>
N:	28
Object:	Poss. SN (SIMBAD class: Supernova_Candidate = SuperNova Candidate)
Stat:	is completely incorporated in Simbad
Note:	VLT VST observations of N=28 sources, in a search for transient counterpart candidates in multi-epoch VST images for GW150914 and GW151226.
Ref:	=2018MNRAS.474..411B
by	BROCATO E. , BRANCHESI M., CAPPELLARO E., COVINO S., GRADO A., GRECO G., LIMATOLA L., STRATTA G., YANG S., CAMPANA S., D'AVANZO P., GETMAN F., MELANDRI A., NICASTRO L., PALAZZI E., PIAN E., PIRANOMONTE S., PULONE L., ROSSI A., TOMASELLA L., AMATI L., ANTONELLI L.A., ASCENZI S., BENETTI S., BULGARELLI A., CAPACCIOLI M., CELLA G., DADINA M., DE CESARE G., D'ELIA V., GHIRLANDA G., GHISELLINI G., GIUFFRIDA G., IANNICOLA G., ISRAEL G., LISI M., LONGO F., MAPELLI M., MARINONI S., MARRESE P., MASETTI N., PATRICELLI B., POSSENTI A., RADOVICH M., RAZZANO M., SALVATERRA R., SCHIPANI P., SPERA M., STAMERRA A., STELLA L., TAGLIAFERRI G., TESTA V., (The GRAWITA: GRAvitational Wave Inaf TeAm)
	Mon. Not. R. Astron. Soc., 474, 411-426 (2018)
	GRAWITA: VLT Survey Telescope observations of the gravitational wave sources GW150914 and GW151226.
o	Text, Tables 4-5: <[BBC2018] VSTJDDD.ddddd+DD.ddddd> N=28.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBC89]
[BBC89]	(Borra+Beauchemin+Crotts+, 1989)
Write:	<<[BBC89] HHMM+DDMMA>> <<[BBC89] HHMMSS.s+DDMMSS>>
N:	36+3
Object:	QSO + G + * (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Note:	Table III: N=33 QSO + 3 G Table V: N=3 WD
Ref:	=1989AJ.....97..344B
by	BORRA E.F. , BEAUCHEMIN M., CROTTS A.P.S., MORTON D.C., YORK D.G.
	Astron. J., 97, 344-356 (1989)
	Spectroscopy of quasar candidates found with slitless spectroscopy.
o	Table III: <[BBC89] HHMM+DDMMA> N=33+3. Table V: <[BBC89] HHMMSS.s+DDMMSS> N=3
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBC91]
[BBC91]	(Brouillet+Baudry+Combes+, 1991)
Write:	<<[BBC91] WNN>> <<[BBC91] WNW>> <<[BBC91] WN-N>> <<[BBC91] Dust N>>
N:	17+4+3+2
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	1st ref., Table 3: 17CO detected positions in the galaxy M 81, (Nos N1-N12) and (S1-S6), No. N8 missing. Two of the South positions have components (Nos S2S, S2N, S2E, S5W) 2nd ref., Table 5: The S2 position is divided into 3 components: (Nos S2-1, S2-2, S2-3) 1st ref., Table 2: N=2 Dust lanes, format 'Dust N'
in source:	M 81 = NGC 3031
Ref:	=1991A&A...242...35B
by	BROUILLET N. , BAUDRY A., COMBES F., KAUFMAN M., BASH F.
	Astron. Astrophys., 242, 35-48 (1991)
	M 81: CO content and interaction with its companion galaxies.
o	Table 3: <[BBC91] WNNW> (Nos N1-N12, S1-S6, S2S, S2N, S2E, S5W). Table 2: <[BBC91] Dust N> (Nos 1-2)
Ref:	=1994A&A...287...20B
by	BAUDRY A. , BROUILLET N., HENKEL C.
	Astron. Astrophys., 287, 20-31 (1994)
	H_{2}O activity in M 82 and in other members of the M 81 group.
o	Table 5: format 'NNN' = [KBK87] NNN
o	Table 2: <BBH Group R> (Nos I to XIII>. Table 5: <BBH IRAS N> (Nos 1-3). Table 5: <[BBC91] WN-N> (Nos S2-1 to S2-3)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBC96]
[BBC96]	(Burbidge+Beaver+Cohen+, 1996)
Write:	<<[BBC96] NN>>
N:	31
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations
in source:	AO 0235+16
Ref:	=1996AJ....112.2533B
by	BURBIDGE E.M. , BEAVER E.A., COHEN R.D., JUNKKARINEN V.T., LYONS R.W.
	Astron. J., 112, 2533-2540 (1996)
	AO 0235+164 and surrounding field: surprising HST results.
o	Table 2: <[BBC96] NN> (Nos 1-31)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BBCDF
BBCDF	(Barbosa+Blum+Conti+Daminelli+Figueredo) (Not yet in Simbad)
Write:	<<BBCDF N>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	NIFS Gemini-North observatory on Mauna Kea observations of [WBN74] W 51 IRS 2.
in source:	W 51:[WBN74] W 51 IRS 2 = [WBN74] W 51 IRS 2
Ref:	=2008ApJ...678L..55B
by	BARBOSA C.L. , BLUM R.D., CONTI P.S., DAMINELI A., FIGUEREDO E.
	Astrophys. J., 678L, 55-58 (2008)
	High spatial resolution spectroscopy of W51 IRS 2E and IRS 2W: two very massive young stars in early formation stages.
o	Fig.1: <BBCDF N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBD2002]
[BBD2002]	(Barbera+Bocchino+Damiani+, 2002)
Write:	<<[BBD2002] PNN>> <<[BBD2002] HNN>> <<[BBD2002] NNNN>>
N:	105
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT PSPC and HRI observations of NGC 2422. PSPC sources have a format 'PNN', HRI sources 'HNN', and sources observed with both PSPC and HRI have also a format 'NNNN' with the first two digit for PSPC. N=105 among 71+45.
in source:	NGC 2422
Ref:	=2002A&A...387..463B
by	BARBERA M. , BOCCHINO F., DAMIANI F., MICELA G., SCIORTINO S., FAVATA F., HARNDEN F.R.Jr
	Astron. Astrophys., 387, 463-478 (2002)
	ROSAT PSPC/HRI observations of the open cluster NGC 2422.
o	Table 1: <[BBD2002] PNN> (Nos P01-P71), <[BBD2002] HNN> (Nos H01-H45), <[BBD2002] NNNN> N=28.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBD2003]
[BBD2003]	(Bica+Bonatto+Dutra, 2003)
Write:	<<[BBD2003] Object N>>
N:	3
Object:	Poss. Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	DSS and 2MASS observations. N=3 cluster candidates in Ass Cyg OB 2. Object 3 does not appear in optical images.
in source:	Ass Cyg OB 2 = NAME VI CYG
Ref:	=2003A&A...405..991B
by	BICA E. , BONATTO C., DUTRA C.M.
	Astron. Astrophys., 405, 991-998 (2003)
	Does Cyg OB2 harbour any open cluster?
o	Do 44 = Cl Dolidze 44.
o	<[BBD2003] Object N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBD2004]
[BBD2004]	(Bica+Bonatto+Dutra, 2004)
Write:	<<[BBD2004] Cluster N>>
N:	3
Object:	Cluster of * (SIMBAD class: OpenCluster = Open Cluster)
Stat:	is completely incorporated in Simbad
Note:	DSS and XDSS images. Analysis based on 2MASS archival data. Discovery of N=3 open clusters in the Milky Way.
Ref:	=2004A&A...422..555B
by	BICA E. , BONATTO C., DUTRA C.M.
	Astron. Astrophys., 422, 555-562 (2004)
	Discovery of three optical open clusters in the Galaxy.
o	Table 1: <[BBD2004] Cluster N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBD2006]
[BBD2006]	(Borys+Blain+Dey+, 2006)= (MIPS)
Write:	<<[BBD2006] MIPS JHHMMSS.s+DDMMSS>> <<[BBD2006] Foreground Galaxy>>
N:	1+1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Observations of a target selected from the Spitzer MIPS instrument with SHARC-II Camera at the Caltech submm observatory: detection of a hyperluminous starburst galaxy. Complementary data from Spitzer IRAC, Keck II, NIRSPEC and DEIMOS, JCMT SCUBA, KPNO 2.1m telescope. Another foreground galaxy is observed.
Ref:	=2006ApJ...636..134B
by	BORYS C. , BLAIN A.W., DEY A., LE FLOC'H E., JANNUZI B.T., BARNARD V., BIAN C., BRODWIN M., MENENDEZ-DELMESTRE K., THOMPSON D., BRAND K., BROWN M.J.I., DOWELL C.D., EISENHARDT P., FARRAH D., FRAYER D.T., HIGDON J., HIGDON S., PHILLIPS T., SOIFER B.T., STERN D., WEEDMAN D.
	Astrophys. J., 636, 134-139 (2006)
	MIPS J142824.0+352619: a hyperluminous starburst galaxy at z = 1.325.
o	Text: <[BBD2006] MIPS JHHMMSS.s+DDMMSS> N=1, <[BBD2006] Foreground Galaxy> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBD2008]
[BBD2008]	(Bica+Bonatto+Dutra, 2008)
Write:	<<[BBD2008] Faint-star clump>> <<[BBD2008] New Cluster N>>
N:	1+3
Object:	Clump + Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Study of stellar clustering in the area of Cl Bochum 1.
Ref:	=2008A&A...489.1129B
by	BICA E. , BONATTO C., DUTRA C.M.
	Astron. Astrophys., 489, 1129-1140 (2008)
	Investigating the borderline between a young star cluster and a small stellar association: a test case with Bochum 1.
o	In paragraph 2 IRAS 06219+2258 is a misprint for IRAS 06219+2001 or IRAS 19403+2258.
o	Fig.1, Table 1: <[BBD2008] Faint-star clump> N=1, <[BBD2008] New Cluster N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBD2019]
[BBD2019]	(Biazzo+Beccari+De Marchi+, 2019)
Write:	<<[BBD2019] [1\|2]NNNNN>>
N:	245
Object:	Poss. PMS* (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=245 PMS star candidates to the stellar association LH 95 in the LMC. Use of HST WFPC2 archival data.
in source:	LH 95
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2019ApJ...875...51B
by	BIAZZO K. , BECCARI G., DE MARCHI G., PANAGIA N.
	Astrophys. J., 875, 51-51 (2019)
	Photometric determination of the mass accretion rates of pre-main-sequence stars. VI. The case of LH 95 in the Large Magellanic Cloud.
o	Table 3: <[BBD2019] 1NNNNN> N=124 among (Nos 100583-105940), <[BBD2019] 2NNNNN> N=121 among (Nos 200884-206419).
=E=	Catalogue in electronic form as <J/ApJ/875/51/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBD74]
[BBD74]	(Barbieri+Bertola+Di tullio, 1974)= (Barbieri)
Write:	<<[BBD74] Blue a>> <<[BBD74] HA N>>
N:	13+4
Object:	Condensation (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Search for main condensations visible in the Blue and in H-alpha in NGC 3077.
in source:	NGC 3077
Ref:	=1974A&A....35..463B
by	BARBIERI C. , BERTOLA F., DI TULLIO G.
	Astron. Astrophys., 35, 463-466 (1974)
	The peculiar galaxy NGC 3077.
o	Table 1: <[BBD74] Blue a> (Nos a-m), <[BBD74] HA N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BBDS
BBDS	(Bica+Bonatto+Dutra+Santos)
Write:	<<BBDS NN>>
N:	10
Object:	Cluster of * + Assoc. + Em. Nebula (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=10 new objects, added to the catalogue of extended objects in the Magellanic System.
in source:	NAME Magellanic Clouds
Ref:	=2008MNRAS.389..678B
by	BICA E. , BONATTO C., DUTRA C.M., SANTOS J.F.C.Jr
	Mon. Not. R. Astron. Soc., 389, 678-690 (2008)
	A general catalogue of extended objects in the Magellanic System.
o	Table 3-5: <BBDS NN> (Nos 1-10).
=E=	Catalogue in electronic form as J/MNRAS/389/678
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BBE90]
[BBE90]	(Beauchemin+Borra+Edwards, 1990)
Write:	<<[BBE90] HHMMSS+DDMMSS>>
N:	758+25
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Note:	Table 5: Format 'HHMMSS+DDMMSS' is the format adopted by the authors in the 2nd ref. The internal 'Gren number' is not used in SIMBAD
Ref:	=1990MNRAS.247..182B
by	BEAUCHEMIN M. , BORRA E.F., EDWARDS G.
	Mon. Not. R. Astron. Soc., 247, 182-199 (1990)
	A homogeneous catalogue of quasar candidates found with slitless spectroscopy.
o	Table 5: <[BBE90] HHMMSS+DDMMSS> N=758
Ref:	=1996AJ....111.1456B
by	BORRA E.F. , LEVESQUE S., BEAUCHEMIN M., MORTON D.C., STOUGHTON C., VANDEN BERK D., YORK D.G., GREEN R.F., CROTTS A.P.S.
	Astron. J., 111, 1456-1497 (1996)
	Spectroscopy of quasar candidates found with slitless spectroscopy. II. Six northern fields.
o	Table 3a: <[BBE90] HHMMSS+DDMMSS> N=25 are new
=E=	Catalogue in electronic form as J/MNRAS/247/182
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBF2004]
[BBF2004]	(Buta+Byrd+Freeman, 2004)
Write:	<<[BBF2004] NN>>
N:	58
Object:	(X) (SIMBAD class: PartofG = Part of a Galaxy)
Note:	HST WFPC2 images of the inner ring of NGC 3081. N=58 sources brighter than V=23.6, likely to be star clusters, massive young stars. A few are foreground stars or background galaxies.
in source:	NGC 3081
Ref:	=2004AJ....127.1982B
by	BUTA R.J. , BYRD G.G., FREEMAN T.
	Astron. J., 127, 1982-2001 (2004)
	A Hubble space telescope study of star formation in the inner resonance ring of NGC 3081.
o	Table 3: <[BBF2004] NN> (Nos 1-58).
=E=	Catalogue in electronic form as J/AJ/127/1982
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBF2008]
[BBF2008]	(Bradley+Bouwens+Ford+, 2008)
Write:	<<[BBF2008] A1689-zD1>>
N:	1
Object:	Grav. lensed image of a G (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=1 strongly lensed Lyman break galaxy candidate in the field of Abell 1689. Use of HST ACS and NICMOS data. Use of Spitzer IRAC data.
in source:	ACO 1689
Ref:	=2008ApJ...678..647B
by	BRADLEY L.D. , BOUWENS R.J., FORD H.C., ILLINGWORTH G.D., JEE M.J., BENITEZ N., BROADHURST T.J., FRANX M., FRYE B.L., INFANTE L., MOTTA V., ROSATI P., WHITE R.L., ZHENG W.
	Astrophys. J., 678, 647-654 (2008)
	Discovery of a very bright strongly lensed galaxy candidate at z ~ 7.6.
o	<[BBF2008] A1689-zD1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBF2014]
[BBF2014]	(Beccari+Bellazzini+Fraternali+, 2014)
Write:	<<[BBF2014] NNNNN>>
N:	12694
Note:	VLT VIMOS deep wide-field photometry of N=12694 stars in the Sagittarius dIrr galaxy. Use of archival HST ACS images.
in source:	NAME Sag dIG
Ref:	=2014A&A...570A..78B
by	BECCARI G. , BELLAZZINI M., FRATERNALI F., BATTAGLIA G., PERINA S., SOLLIMA A., OOSTERLOO T.A., TESTA V., GALLETI S.
	Astron. Astrophys., 570A, 78-78 (2014)
	The extended structure of the dwarf irregular galaxy Sagittarius.
o	in6.dat: <[BBF2014] NNNNN> N=12694 among (Nos 1-14823).
=E=	Catalogue in electronic form as J/A+A/570/A78
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBF84]
[BBF84]	(Battistini+Bonoli+Federici+, 1984)
Write:	<<[BBF84] FNN>>
N:	15
Object:	Poss. GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	N=15 globular clusters candiates in NGC 2403.
in source:	NGC 2403
Ref:	=1984A&A...130..162B
by	BATTISTINI P. , BONOLI F., FEDERICI L., FUSI PECCI F., KRON R.G.
	Astron. Astrophys., 130, 162-166 (1984)
	Globular cluster candidates in the spiral galaxy NGC 2403.
o	Table 2: 'CN' = TS CN in SIMBAD.
o	Fig.1, Table 2: <[BBF84] FNN> N=15 among (Nos F1-F47).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BBG
BBG	(Balmer Break Galaxy)
Write:	<<BBG NNNN>>
N:	13
Object:	G (SIMBAD class: Galaxy)
Note:	HST ACS, VLT ISAAC, and Spitzer IRAC observations in the GOODS South Field. Search for massive evolved galaxies at z > about 5.
in source:	NAME GOODS South Field
Ref:	=2008ApJ...676..781W
by	WIKLIND T. , DICKINSON M., FERGUSON H.C., GIAVALISCO M., MOBASHER B., GROGIN N.A., PANAGIA N.
	Astrophys. J., 676, 781-806 (2008)
	A population of massive and evolved galaxies at z≳5.
o	Table 2: <BBG NNNN> N=13 among (Nos 547-5197).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BBG2007]
[BBG2007]	(Barrena+Boschin+Girardi+, 2007)= ([BBG2007a])
Write:	<<[BBG2007] NNN>> <<[BBG2007] FNNN>> <<[BBG2007] JHHMMSS.s+DDMMSS>>
N:	142
Object:	G in ClG (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	TNG telescope spectroscopy of galaxies in ACO 773. Format 'NNN' for galaxy members of the cluster, 'FNNN' for galaxies in the field of the cluster.
in source:	ACO 773
Ref:	=2007A&A...467...37B
by	BARRENA R. , BOSCHIN W., GIRARDI M., SPOLAOR M.
	Astron. Astrophys., 467, 37-48 (2007)
	Internal dynamics of the radio halo cluster Abell 773: a multiwavelength analysis.
o	Dominant galaxies D1 and D2 are respectively [BBG2007] 59 AND 60.
o	Table 1: <[BBG2007] NNN> or <[BBG2007] FNNN> N=100+42.
=E=	Catalogue in electronic form as J/A+A/467/37
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBG2007a]
[BBG2007a]	(Barrena+Boschin+Girardi+, 2007)
*****	Avoid the usage of [BBG2007a], prefer [BBG2007]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBG2007b]
[BBG2007b]	(Barrena+Boschin+Girardi+, 2007)
Write:	<<[BBG2007b] NNN>> <<[BBG2007b] NNNF>> <<[BBG2007b] JHHMMSS.s+DDMMSS>>
N:	115
Object:	G in ClG (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	TNG spectroscopy of galaxies in ACO 115. Format 'NNN' for cluster members, 'NNNF' for galaxies in the field of the cluster.
in source:	ACO 115
Ref:	=2007A&A...469..861B
by	BARRENA R. , BOSCHIN W., GIRARDI M., SPOLAOR M.
	Astron. Astrophys., 469, 861-872 (2007)
	The dynamical status of the galaxy cluster Abell 115.
o	Table 1: <[BBG2007b] NNN> or <[BBG2007b] NNNF> (Nos 1-115) = <[BBG2007b] JHHMMSS.s+DDMMSS> N=115.
=E=	Catalogue in electronic form as J/A+A/469/861
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBG2008]
[BBG2008]	(Boschin+Barrena+Girardi+, 2008)
Write:	<<[BBG2008] ACO 610 NNN>> <<[BBG2008] ACO 725 NN>> <<[BBG2008] ACO 796 NN>>
N:	165+51+99
Object:	G (SIMBAD class: Galaxy)
Note:	WHT WYFFOS spectroscopy and INT WFC photometry of N=3 galaxy clusters.
in source:	ACO 610
in source:	ACO 725
in source:	ACO 796
Ref:	=2008A&A...487...33B
by	BOSCHIN W. , BARRENA R., GIRARDI M., SPOLAOR M.
	Astron. Astrophys., 487, 33-46 (2008)
	Optical analysis of the poor clusters Abell 610, Abell 725, and Abell 796, containing diffuse radio sources.
o	Table 1, Fig.2: <[BBG2008] ACO 610 NNN> (Nos 1-165). Table 4, Fig.12: <[BBG2008] ACO 725 NN> (Nos 1-51). Table 5, Fig.16: <[BBG2008] ACO 796 NN> (Nos 1-99).
=E=	Catalogue in electronic form as J/A+A/487/33
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBG2009]
[BBG2009]	(Boschin+Barrena+Girardi, 2009)
Write:	<<[BBG2009] NNN>>
N:	107
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	TNG spectroscopy of galaxies in ACO 959.
in source:	ACO 959
Ref:	=2009A&A...495...15B
by	BOSCHIN W. , BARRENA R., GIRARDI M.
	Astron. Astrophys., 495, 15-26 (2009)
	Internal dynamics of the galaxy cluster Abell 959.
o	Paragraph.4 NVSS J101642+592222 is NVSS J101636+592210 in Simbad.
o	Table 1, Fig. 2: <[BBG2009] NNN> (Nos 1-107).
=E=	Catalogue in electronic form as J/A+A/495/15
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBG2010]
[BBG2010]	(Boudreault+Bailer-Jones+Goldman+, 2010)= (Praesepe) = ([BBG2010a])
Write:	<<[BBG2010] NNN>>
N:	124+27
Object:	Brown Dwarf + Low Mass * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Calar Alto 3.5m telescope and MPG/ESO 2.2m telescope WFI observations of the Praesepe open cluster.
in source:	NAME Praesepe
Ref:	=2010A&A...510A..27B
by	BOUDREAULT S. , BAILER-JONES C.A.L., GOLDMAN B., HENNING T., CABALLERO J.A.
	Astron. Astrophys., 510A, 27-27 (2010)
	Brown dwarfs and very low mass stars in the Praesepe open cluster: a dynamically unevolved mass function?
o	Table 3: <[BBG2010] NNN> (Nos 1-124), <[BBG2010] 9NN> (Nos 901-927).
=E=	Catalogue in electronic form as J/A+A/510/A27
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBG2010a]
[BBG2010a]	(Boudreault+Bailer-Jones+Goldman+, 2010)= (Praesepe)
Note:	Calar Alto 3.5m telescope and MPG/ESO 2.2m telescope WFI observations
*****	Avoid the usage of [BBG2010a], prefer [BBG2010]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBG2010b]
[BBG2010b]	(Bettoni+Buson+Galletta, 2010)
Write:	<<[BBG2010b] Clump N>>
N:	6
Object:	Clump (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	GALEX observations of N=6 UV-bright clumps surrounding NGC 4262.
in source:	NGC 4262
Ref:	=2010A&A...519A..72B
by	BETTONI D. , BUSON L.M., GALLETTA G.
	Astron. Astrophys., 519A, 72-72 (2010)
	NGC 4262: a Virgo galaxy with an extended ultraviolet ring.
o	Fig. 6, Table 2: <[BBG2010b] Clump N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBG2010c]
[BBG2010c]	(Boschin+Barrena+Girardi, 2010)
Write:	<<[BBG2010c] NNN>>
N:	125
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	TNG and INT observations of N=125 galaxies in ACO 2345.
in source:	ACO 2345
Ref:	=2010A&A...521A..78B
by	BOSCHIN W. , BARRENA R., GIRARDI M.
	Astron. Astrophys., 521A, 78-78 (2010)
	The complex structure of Abell 2345: a galaxy cluster with non-symmetric radio relics.
o	Table 1: <[BBG2010c] NNN> (Nos 1-125).
=E=	Catalogue in electronic form as J/A+A/521/A78
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBG2011]
[BBG2011]	(Burgasser+Bardalez-Gagliuffu+Gizis+, 2011)= ([BBG2011a]) (Not yet in Simbad)
Write:	<<[BBG2011] 2MASS J1728+3948>> <<[BBG2011] 2MASS J1728+3948A>>
N:	1+2
Object:	** + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	IRTF SpeX spectroscopic observations of 2MASS J17281150+3948593. See also [FBB2011].
Ref:	=2011AJ....141...70B
by	BURGASSER A.J. , BARDALEZ-GAGLIUFFI D.C., GIZIS J.E.
	Astron. J., 141, 70 (2011)
	Hubble space telescope imaging and spectral analysis of two brown dwarf binaries at the L dwarf/T dwarf transition.
o	<[BBG2011] 2MASS J1728+3948> N=1, <[BBG2011] 2MASS J1728+3948A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBG2011a]
[BBG2011a]	(Burgasser+Bardalez-Gagliuffu+Gizis+, 2011) (Not yet in Simbad)
*****	Avoid the usage of [BBG2011a], prefer [BBG2011]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBG2011b]
[BBG2011b]	(Battersby+Bally+Ginsburg+, 2011)
Write:	<<[BBG2011b] EGO GLLL.ll+BB.bb>> <<[BBG2011b] GLLL.ll+BB.bb>>
N:	8+5
Object:	* + Poss. IRDC (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=8 EGO (Extended Green Object) candidates and N=5 IRDC (Infrared Dark Cloud) candidates. Use of data from the Hi-GAL (Herschel Infrared GALactic plane) survey and of archival Spitzer data.
Ref:	=2011A&A...535A.128B
by	BATTERSBY C. , BALLY J., GINSBURG A., BERNARD J.-P., BRUNT C., FULLER G.A., MARTIN P., MOLINARI S., MOTTRAM J., PERETTO N., TESTI L., THOMPSON M.A.
	Astron. Astrophys., 535A, 128-128 (2011)
	Characterizing precursors to stellar clusters with Herschel.
o	Fig. 8, Table 1: <[BBG2011b] EGO GLLL.ll+BB.bb> N=8. Table 4: <[BBG2011b] GLLL.ll+BB.bb> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBG2017]
[BBG2017]	(Bitsakis+Bonfini+Gonzalez-Lopezlira+, 2017)
Write:	<<[BBG2017] IR1-NNNN>> <<[BBG2017] M2-NNNN>> <<[BBG2017] NUV-NNNN>> <<[BBG2017] IR1_NNNN>> (not recognised by Simbad, but found in literature) <<[BBG2017] M2_NNNN>> <<[BBG2017] NUV_NNNN>>
N:	2373+741+736
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	N=4850 star clusters in the Large Magellanic Cloud. Use of archival data from GALEX, SUMAC survey (Swift/UVOT Magellanic Clouds Survey), MCPS survey (Magellanic Cloud Photometric Survey), and Spitzer SAGE. See also [BGB2018].
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2017ApJ...845...56B
by	BITSAKIS T. , BONFINI P., GONZALEZ-LOPEZLIRA R.A., RAMIREZ-SIORDIA V.H., BRUZUAL G., CHARLOT S., MARAVELIAS G., ZARITSKY D.
	Astrophys. J., 845, 56-56 (2017)
	A novel method to automatically detect and measure the ages of star clusters in nearby galaxies: application to the Large Magellanic Cloud.
o	Table 2: <[BBG2017] IR1-NNNN> N=2373 among (Nos IR1-1 to IR1-2653), <[BBG2017] M2-NNNN> N=741 among (Nos M2-3 to M2-1294), <[BBG2017] NUV-NNNN> N=1736 among (Nos NUV-2 to NUV-2334).
=E=	Catalogue in electronic form as <J/ApJ/845/56/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BBH
BBH	(Baudry+Brouillet+Henkel)= (IRAS)
Write:	<<BBH Group R>> <<BBH IRAS N>>
N:	13+3
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=13 features identified in the H2O maser spectra, (Nos I to XIII) Table 5: N=3 (IR) components, format 'IRAS N'
in source:	M 81 = NGC 3031
Ref:	=1994A&A...287...20B
by	BAUDRY A. , BROUILLET N., HENKEL C.
	Astron. Astrophys., 287, 20-31 (1994)
	H_{2}O activity in M 82 and in other members of the M 81 group.
o	Table 5: format 'NNN' = [KBK87] NNN
o	Table 2: <BBH Group R> (Nos I to XIII>. Table 5: <BBH IRAS N> (Nos 1-3). Table 5: <[BBC91] WN-N> (Nos S2-1 to S2-3)
Origin	of the Acronym: L (1996A&A...316..188B)
Details on Acronym: [BBH2003]
[BBH2003]	(Boeche+Barbon+Henden+, 2003)
Write:	<<[BBH2003] NN>>
N:	30
Object:	* (SIMBAD class: Star)
Note:	Stars in the field of NGC 6738.
in source:	NGC 6738
Ref:	=2003A&A...406..893B
by	BOECHE C. , BARBON R., HENDEN A., MUNARI U., AGNOLIN P.
	Astron. Astrophys., 406, 893-898 (2003)
	NGC 6738: Not a real open cluster.
o	Fig.1, Table 2: <[BBH2003] NN> (Nos 1-30).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBH2005]
[BBH2005]	(Boone+Brouillet+Huttemeister+, 2005)
Write:	<<[BBH2005] HII>> <<[BBH2005] BN>> <<[BBH2005] RN>> <<[BBH2005] Concentration R>> <<[BBH2005] MC>>
N:	1+6+2+2+1
Object:	Feature (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	CFHT B, R, and Halpha imaging of the region of Holmberg IX.
Ref:	=2005A&A...429..129B
by	BOONE F. , BROUILLET N., HUETTEMEISTER S., HENKEL C., BRAINE J., BOMANS D.J., HERPIN F., BANHIDI Z., ALBRECHT M.
	Astron. Astrophys., 429, 129-140 (2005)
	Properties and environment of the molecular complex near Holmberg IX.
o	Fig.5: new small HII region = EQ J095758.6+690319.0 in SIMBAD. Fig.10: Molecular Complex 'MC' = NAME MOLECULAR COMPLEX NEAR Ho IX in SIMBAD.
o	Fig.5: <[BBH2005] HII> N=1. Figs 6, 7: <[BBH2005] AN> (Nos B1-B6, R1-R2). Fig.8: <[BBH2005] Concentration R> (Nos I, II). Fig.10: <[BBH2005] MC> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBH2019]
[BBH2019]	(Britavskiy+Bonanos+Herrero+, 2019)
Write:	<<[BBH2019] IC NNNN N>> <<[BBH2019] Pegasus N>> <<[BBH2019] Phoenix 3>> <<[BBH2019] Sextans A NN>> <<[BBH2019] Sextans B N>> <<[BBH2019] WLM 1N>>
N:	6+3+2+1+7+2+4
Object:	Poss. Red Supergiant (SIMBAD class: RedSG_Candidate = Red Supergiant Candidate)
Stat:	is completely incorporated in Simbad
Note:	Gran Telescopio Canarias OSIRIS and VLT FORS2 observations of N=25 red supergiant candidates in star-forming dIrr galaxies in the Local Group. See also [BBM2014] and [BBM2015].
in source:	IC 10
in source:	IC 1613
in source:	NAME Pegasus Galaxy
in source:	NAME Phe Galaxy
in source:	DDO 75 = NAME Sextans A
in source:	DDO 70 = NAME Sextans B
in source:	NAME WLM Galaxy
Ref:	=2019A&A...631A..95B
by	BRITAVSKIY N.E. , BONANOS A.Z., HERRERO A., CERVINO M., GARCIA-ALVAREZ D., BOYER M.L., MASSERON T., MEHNER A., McQUINN K.B.W.
	Astron. Astrophys., 631A, 95-95 (2019)
	Physical parameters of red supergiants in dwarf irregular galaxies in the Local Group.
o	Table 3: <[BBH2019] IC 10 N> (Nos 1-6), <[BBH2019] IC 1613 N> (Nos 1-3), <[BBH2019] Pegasus N> (Nos 1-2), <[BBH2019] Phoenix 3> N=1, <[BBH2019] Sextans A NN> (Nos 4-10), <[BBH2019] Sextans B N> (Nos 1-2), <[BBH2019] WLM NN> (Nos 11-14).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [BBH97]
[BBH97]	(Borkowski+Blondin+Harrington, 1997) (Not yet in Simbad)
Write:	<<[BBH97] WWNa>>
N:	6+3+3
Object:	Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST WFPC2 observations of Hen 3-1475. Knots and subcondensations in knots in the jet of Hen 3-1475.
in source:	Hen 3-1475
Ref:	=1997ApJ...482L..97B
by	BORKOWSKI K.J. , BLONDIN J.M., HARRINGTON J.P.
	Astrophys. J., 482, 97-100 (1997)
	Collimation of astrophysical jets: the proto-planetary nebula He 3-1475.
o	Fig.2: <[BBH97] WWN> (Nos SE1 to SE3, NW1 to NW3).
Ref:	=2002RMxAC..13..127R
by	RIERA A. , GARCIA-LARIO P., MANCHADO A., BOBROWSKY M., ESTALELLA R.
	Rev. Mex. Astron. Astrofis. Serie de Conf., 13, 127-132 (2002)
	New observations of the high-velocity outflows of the proto-planetary nebula Hen 3-1475.
o	Fig.1, Table 1: <[BBH97] WWWNa> (Nos SE1a to SE1c) added.
Ref:	=2003A&A...401.1039R
by	RIERA A. , GARCIA-LARIO P., MANCHADO A., BOBROWSKY M., ESTALELLA R.
	Astron. Astrophys., 401, 1039-1056 (2003)
	The high-velocity outflow in the proto-planetary nebula Hen 3-1475.
o	Fig.1, Table 1: <[BBH97] WWWNa> (Nos NW1a to NW1c) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBH99]
[BBH99]	(Barkana+Blandford+Hogg, 1999)= (HDFS)
Write:	<<[BBH99] HDFS JHHMMSSs-DDMMSS>> <<[BBH99] Arc A>> <<[BBH99] Dot>>
N:	1+4+1
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	The gravitational lens system 'HDFS J2232509-603243' (truncated format J22325090, not rounded) has the morphology of an elliptical galaxy with a much bluer arc, the arc being separated into 4 components A to D. There is also a faint point-like source named the 'Dot'
in source:	NAME HDFS
Ref:	=1999ApJ...513L..91B
by	BARKANA R. , BLANDFORD R., HOGG D.W.
	Astrophys. J., 513, 91-94 (1999)
	A possible gravitational lens in the Hubble Deep Field South.
o	Table 2: <[BBH99] HDFS J2232509-603243> N=1, <[BBH99] Arc A> (Nos A-D), <[BBH99] Dot> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BBJ
BBJ	(Beccari+Boffin+Jerabkova) (Not yet in Simbad)
*****	Avoid the usage of BBJ, prefer [BBJ2020]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BBJ2010]
[BBJ2010]	(Battersby+Bally+Jackson+, 2010)
Write:	<<[BBJ2010] MSXDC GLLL.ll+BB.bb GLMN>> <<[BBJ2010] MSXDC GLLL.ll+BB.bb VLAN>>
N:	17+16
Object:	Clump + (Rad) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HHT (HCO+ and N2H+), CSO (1.1mm), and VLA (3.6cm) observations. Use of BU-FCRAO GR, Spitzer GLIMPSE and MIPSGAL data.
Ref:	=2010ApJ...721..222B
by	BATTERSBY C. , BALLY J., JACKSON J.M., GINSBURG A., SHIRLEY Y.L., SCHLINGMAN W., GLENN J.
	Astrophys. J., 721, 222-250 (2010)
	An infrared through radio study of the properties and evolution of IRDC clumps.
o	Tables 1, 3-5: <[BBJ2010] MSXDC GLLL.ll+BB.bb GLMN> N=17. Table 6: <[BBJ2010] MSXDC GLLL.ll+BB.bb VLAN> N=16.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBJ2018]
[BBJ2018]	(Beccari+Boffin+Jerabkova+, 2018)
Write:	<<[BBJ2018] N>>
N:	6
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	ESO VST 2.4-m OmegaCAM photometric observations of N=6 clusters in the field of the Wolf–Rayet Star γ^2 Vel. Use of archival GAIA data.
Ref:	=2018MNRAS.481L..11B
by	BECCARI G. , BOFFIN H.M.J., JERABKOVA T., WRIGHT N.J., KALARI V.M., CARRARO G., DE MARCHI G., DE WIT W.-J.
	Mon. Not. R. Astron. Soc., 481L, 11 (2018)
	A sextet of clusters in the Vela OB2 region revealed by Gaia.
o	Table 1: <[BBJ2018] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBJ2020]
[BBJ2020]	(Beccari+Boffin+Jerabkova, 2020)= (BBJ)
Write:	<<[BBJ2020] N>>
N:	3
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	N=3 star clusters identified in Gaia DR2 data.
Ref:	=2020MNRAS.491.2205B
by	BECCARI G. , BOFFIN H.M.J., JERABKOVA T.
	Mon. Not. R. Astron. Soc., 491, 2205-2216 (2020)
	Uncovering a 260 pc wide, 35-Myr-old filamentary relic of star formation.
o	Fig. 6: <[BBJ2020] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBK2000]
[BBK2000]	(Brown+Bowers+Kimble+, 2000)
Write:	<<[BBK2000] JHHMMSS.ssss+DDMMSS.sss>>
N:	about 8000
Object:	* (SIMBAD class: Star)
Note:	HST STIS observations. Stars observed in the near-UV in M 32.
in source:	M 32
Ref:	=2000ApJ...532..308B
by	BROWN T.M. , BOWERS C.W., KIMBLE R.A., SWEIGART A.V., FERGUSON H.C.
	Astrophys. J., 532, 308-322 (2000)
	Detection and photometry of hot horizontal branch stars in the core of M32.
o	Table 1: <[BBK2000] JHHMMSS.ssss+DDMMSS.sss> N=about 8000.
=E=	Catalogue in electronic form as J/ApJ/532/308
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBK2005]
[BBK2005]	(Bolton+Burles+Koopmans+, 2005)
Write:	<<[BBK2005] A>>
N:	4
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Stat:	is completely incorporated in Simbad
Note:	Gemini spectroscopy and HST images of a four-image gravitational lens: SDSS J140228.22+632133.3. The lensed object is [BBS2004] BG 0.4814.
Ref:	=2005ApJ...624L..21B
by	BOLTON A.S. , BURLES S., KOOPMANS L.V.E., TREU T., MOUSTAKAS L.A.
	Astrophys. J., 624, 21-24 (2005)
	SDSS J140228.22+632133.3: a new spectroscopically selected gravitational lens.
o	Fig.1: <[BBK2005] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBK2006]
[BBK2006]	(Ben Bekhti+Bruns+Kerp+, 2006) (Not yet in Simbad)
Write:	<<[BBK2006] HVC LLL+BB+VVV A>>
N:	20+17
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Note:	ATCA observations of 2 HVC clouds.
in source:	HVC 297+09+253
in source:	HVC 291+26+195
Ref:	=2006A&A...457..917B
by	BEN BEKHTI N. , BRUENS C., KERP J., WESTMEIER T.
	Astron. Astrophys., 457, 917-926 (2006)
	Physical properties of two compact high-velocity clouds possibly associated with the leading arm of the Magellanic system.
o	Table 1: <[BBK2006] HVC 297+09+253 A> (Nos A-T). Table 2: <[BBK2006] HVC 291+26+195 A> (Nos A-Q).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBK2019]
[BBK2019]	(Bayandina+Burns+Kurtz+, 2019)
Write:	<<[BBK2019] VLA N>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA continuum observations of N=4 radio sources in the star-forming region GAL 025.65+01.05.
in source:	GAL 025.65+01.05
Ref:	=2019ApJ...884..140B
by	BAYANDINA O.S. , BURNS R.A., KURTZ S.E., SHAKHVOROSTOVA N.N., VAL'TTS I.E.
	Astrophys. J., 884, 140-140 (2019)
	VLA overview of the bursting H_{2}O maser source G25.65+1.05.
o	Table 2: <[BBK2019] VLA N> (Nos 1-4).
=E=	Catalogue in electronic form as <J/ApJ/884/140/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBK88]
[BBK88]	(Bergeron+Boulade+Kunth+, 1988)
Write:	<<[BBK88] NN>>
N:	22
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Objects in the field of PHL 1226 Map in Fig.3 See also [B86b], [BB86b], [BDK87], [B88], [BB91], [BCS92], [GB97]
Ref:	=1988A&A...191....1B
by	BERGERON J. , BOULADE O., KUNTH D., TYTLER D., BOKSENBERG A., VIGROUX L.
	Astron. Astrophys., 191, 1-9 (1988)
	Crowding on the sight line to the QSO PHL 1226: the nearby galaxy IC 1746 and a galaxy cluster at Z=0.16.
o	Table 4: <[BBK88] NN> (Nos 1-22)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBK99]
[BBK99]	(Bowyer+Berghofer+Korpela, 1999)
Write:	<<[BBK99] JHHMMSS.s+DDMMSS>>
N:	1
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	EUVE observations: Extragal source
Ref:	=1999ApJ...526..592B
by	BOWYER S. , BERGHOEFER T.W., KORPELA E.J.
	Astrophys. J., 526, 592-598 (1999)
	Extreme-ultraviolet emission in Abell 1795, Abell 2199, and the Coma cluster.
o	<[BBK99] JHHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBL2002]
[BBL2002]	(Bremer+Baker+Lehnert, 2002)
Write:	<<[BBL2002] Group>> <<[BBL2002] GN>>
N:	1+5
Object:	Group of G + G (SIMBAD class: Galaxy)
Note:	Discovery of an unusual compact group of galaxies associated with the QSO MRC 0941-200.
Ref:	=2002MNRAS.337..470B
by	BREMER M.N. , BAKER J.C., LEHNERT M.D.
	Mon. Not. R. Astron. Soc., 337, 470-476 (2002)
	A quasar in a compact group of galaxies at z = 0.7.
o	Fig.1, text: <[BBL2002] Group> N=1, <[BBL2002] GN> (Nos G1-G5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBL2003]
[BBL2003]	(Boles+Beutler+Li+, 2003)= ([BBL2003a])
Write:	<<[BBL2003] JHHMMSS.ss+DDMMSS.s>>
N:	4
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxies of SN 2003BX, SN 2003BY, SN 2003BZ, and SN 2003CA.
Ref:	=2003IAUC.8093....1B
by	BOLES T. , BEUTLER B., LI W., BECKER A., (The Deep Lens Survey Team), LOOMBA D., WILCOX R., SCHWARTZ M.
	IAU Circ., 8093, 1-None (2003)
	Supernovae 2003bv, 2003bw, 2003bx, 2003by, 2003bz, 2003ca.
o	<[BBL2003] JHHMMSS.ss+DDMMSS.s> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBL2003a]
[BBL2003a]	(Boles+Beutler+Li+, 2003)
*****	Avoid the usage of [BBL2003a], prefer [BBL2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBL2003b]
[BBL2003b]	(Bauer+Brandt+Lehmer, 2003)
Write:	<<[BBL2003b] NN>> <<[BBL2003b] IC 342 X-N>>
N:	35
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton observations of IC 342. 31 sources among the 35 are plausibly associated with IC 342. The 3 brightest sources are also designated as 'IC 342 X-N'.
in source:	IC 342
Ref:	=2003AJ....126.2797B
by	BAUER F.E. , BRANDT W.N., LEHMER B.
	Astron. J., 126, 2797-2805 (2003)
	The X-ray properties of the nearby star-forming galaxy IC 342: the XMM-newton view.
o	Fig.1, Table 1: <[BBL2003b] NN> (Nos 1-35), <[BBL2003b] IC 342 X-N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBL2010]
[BBL2010]	(Bigiel+Bolatto+Leroy+, 2010)
Write:	<<[BBL2010] N>>
N:	8
Object:	Giant MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	CARMA CO(1-0) observations of N=8 giant molecular clouds in the outer disk of M33.
in source:	M 33 = NGC 598
Ref:	=2010ApJ...725.1159B
by	BIGIEL F. , BOLATTO A.D., LEROY A.K., BLITZ L., WALTER F., ROSOLOWSKY E.W., LOPEZ L.A., PLAMBECK R.L.
	Astrophys. J., 725, 1159-1164 (2010)
	Unusually luminous giant molecular clouds in the outer disk of M33.
o	Fig. 1, Table 1: <[BBL2010] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBL92]
[BBL92]	(Black+Baum+Leahy+, 1992)
Write:	<<[BBL92] 3C NNN.N A>> <<[BBL92] 3C NNN.N AN>>
N:	17+84
Object:	(Rad) (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Figs 1-25: Spots in 3C radio-sources. In the format, the letter P stands for a component Preceding end of the source, F following end of the source, N North of the source, S South of the source, and C Center of the source. Each component is divided into several sub-components 'AN' Paper I, see also Paper II: [LBD97b]
Ref:	=1992MNRAS.256..186B
by	BLACK A.R.S. , BAUM S.A., LEAHY J.P., PERLEY R.A., RILEY J.M., SCHEUER P.A.G.
	Mon. Not. R. Astron. Soc., 256, 186-208 (1992)
	A study of FRII radio galaxies with z<0.15. I. High-resolution maps of eight sources at 3.6 cm.
o	Figs 1-25: <[BBL92] 3C NNN A>, <[BBL92] 3C NNN.N A>, <[BBL92] 3C NNN AN>, <[BBL92] 3C NNN.N AN>, N=17+84.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBL98]
[BBL98]	(Berghofer+Bowyer+Lieu+, 1998)= (lb)
Write:	<<[BBL98] lb LLL+BB>>
N:	3
Object:	Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	EUVE Deep Survey telescope observations Table 2: EUV absorbant clouds
Ref:	=1998ApJ...500..838B
by	BERGHOEFER T.W. , BOWYER S., LIEU R., KNUDE J.
	Astrophys. J., 500, 838-846 (1998)
	The thermal pressure of the hot interstellar medium derived from cloud shadows in the extreme ultraviolet.
o	Table 2: <[BBL98] lb LLL+BB> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BBM
BBM	(Beichman+Boulanger+Moshir)
*****	Avoid the usage of BBM, prefer [BBM92]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [BBM2004]
[BBM2004]	(Boles+Bode+Marchant+, 2004)
Write:	<<[BBM2004] JHHMMSS.s+DDMMSS>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of SN 2004DQ.
Ref:	=2004IAUC.8384....1B
by	BOLES T. , BODE M., MARCHANT J., NEWSAM A.
	IAU Circ., 8384, 1-None (2004)
	Supernova 2004dq.
o	<[BBM2004] JHHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBM2006]
[BBM2006]	(Brosch+Bar-Or+Malka, 2006)= ([BBM2006a])
Write:	<<[BBM2006] JHHMMSS+DDMMSS>>
N:	6+3+11
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Candidate neighbour galaxies in 3 fields.
Ref:	=2006MNRAS.368..864B
by	BROSCH N. , BAR-OR C., MALKA D.
	Mon. Not. R. Astron. Soc., 368, 864-876 (2006)
	Neighbourhoods of isolated star forming dwarf galaxies.
o	Table 4: <[BBM2006] JHHMMSS+DDMMSS> N=6+3+11.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBM2006a]
[BBM2006a]	(Brosch+Bar-Or+Malka, 2006)
*****	Avoid the usage of [BBM2006a], prefer [BBM2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBM2006b]
[BBM2006b]	(Beaulieu+Buchler+Marquette+, 2006)
Write:	<<[BBM2006b] A>>
N:	5
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Stat:	is completely incorporated in Simbad
Note:	Identification of N=5 F-O1-type Beat Cepheids in M 33 from the CFHT variability survey.
in source:	M 33 = NGC 598
Ref:	=2006ApJ...653L.101B
by	BEAULIEU J.-P. , BUCHLER J.R., MARQUETTE J.-B., HARTMAN J.D., SCHWARZENBERG-CZERNY A.
	Astrophys. J., 653L, 101-104 (2006)
	Detection of beat cepheids in M 33 and their use as a probe of the M 33 metallicity distribution.
o	Table 1: <[BBM2006b] A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBM2014]
[BBM2014]	(Britavskiy+Bonanos+Mehner+, 2014)
Write:	<<[BBM2014] Sex A N>> <<[BBM2014] IC1613 N>>
N:	6+2
Object:	RGB* (SIMBAD class: RGB* = Red Giant Branch star)
Stat:	is completely incorporated in Simbad
Note:	Gran Telescopio Canarias OSIRIS and LCO 2.5m du Pont telescope observations of N=6 and N=2 red supergiant stars in Sextans A and IC 1613. See also [BBM2015] and [BBH2019].
in source:	Sextans A = DDO 75
in source:	IC 1613
Ref:	=2014A&A...562A..75B
by	BRITAVSKIY N.E. , BONANOS A.Z., MEHNER A., GARCIA-ALVAREZ D., PRIETO J.L., MORRELL N.I.
	Astron. Astrophys., 562A, 75-75 (2014)
	Identification of red supergiants in nearby galaxies with mid-IR photometry.
o	Tables 1-2: <[BBM2014] Sex A N> (Nos 1-6), <[BBM2014] IC1613 N> (Nos 1-2).
=E=	Catalogue in electronic form as J/A+A/562/A75
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBM2015]
[BBM2015]	(Britavskiy+Bonanos+Mehner+, 2015)
Write:	<<[BBM2015] Phoenix NN>> <<[BBM2015] Pegasus NN>> <<[BBM2015] Sextans A NN>> <<[BBM2015] WLM NN>>
N:	14+19+15+31
Object:	(Mid IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	VLT FORS2 multi-object spectroscopy of N=14+19+15+31 point sources in four star-forming dwarf irregular galaxies: Pegasus, Phoenix,Sextans A and WLM. Use of Spitzer IRAC data. See also [BBM2014] and [BBH2019].
in source:	NAME WLM Galaxy
in source:	NAME Sextans A
in source:	NAME Pegasus Dwarf Galaxy
in source:	NAME Phe Galaxy
Ref:	=2015A&A...584A..33B
by	BRITAVSKIY N.E. , BONANOS A.Z., MEHNER A., BOYER M.L., McQUINN K.B.W.
	Astron. Astrophys., 584A, 33-33 (2015)
	Identification of dusty massive stars in star-forming dwarf irregular galaxies in the Local Group with mid-IR photometry.
o	Table A.1: <[BBM2015] Phoenix NN> (Nos 1-14). Table A.2: <[BBM2015] Pegasus NN> (Nos 1-19). Table A.3: <[BBM2015] Sextans A NN> (Nos 1-15). Table A.4: <[BBM2015] WLM NN> (Nos 1-31).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBM2017]
[BBM2017]	(Beccari+Bellazzini+Magrini+, 2017)
Write:	<<[BBM2017] MBNN>> <<[BBM2017] SBNN>>
N:	26+12
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	VLT MUSE observations of N=26+12 HII regions in the main (MB) and secondary (SB) bodies respectively of the faint star-forming system SECCO 1.
in source:	NAME SECCO 1
Ref:	=2017MNRAS.465.2189B
by	BECCARI G. , BELLAZZINI M., MAGRINI L., COCCATO L., CRESCI G., FRATERNALI F., DE ZEEUW P.T., HUSEMANN B., IBATA R., BATTAGLIA G., MARTIN N., TESTA V., PERINA S., CORRENTI M.
	Mon. Not. R. Astron. Soc., 465, 2189-2197 (2017)
	A very dark stellar system lost in Virgo: kinematics and metallicity of SECCO 1 with MUSE.
o	(Erratum) erratum vol. 468, p. 4254 (2017)
o	Table 1: <[BBM2017] MBNN> N=26 among (Nos MB14-MB68), <[BBM2017] SBNN> N=12 among (Nos SB01-SB45).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBM2018]
[BBM2018]	(Bhandari+Bannister+Murphy+, 2018)
Write:	<<[BBM2018] JHHMMSS+DDMMSS>>
N:	9
Object:	Variable Radio Source (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ASKAP 1.4GHz continuum observations of N=9 variable radio sources in a field centered on the NGC 7232 galaxy group.
Ref:	=2018MNRAS.478.1784B
by	BHANDARI S. , BANNISTER K.W., MURPHY T., BELL M., RAJA W., MARVIL J., HANCOCK P.J., WHITING M., FLYNN C.M., COLLIER J.D., KAPLAN D.L., ALLISON J.R., ANDERSON C., HEYWOOD I., HOTAN A., HUNSTEAD R., LEE-WADDELL K., MADRID J.P., McCONNELL D., POPPING A., RHEE J., SADLER E., VORONKOV M.A.
	Mon. Not. R. Astron. Soc., 478, 1784-1794 (2018)
	A pilot survey for transients and variables with the Australian Square Kilometre Array Pathfinder.
o	Table 3: <[BBM2018] JHHMMSS+DDMMSS> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBM92]
[BBM92]	(Beichman+Boulanger+Moshir, 1992)= (BBM)
Write:	<<[BBM92] NN>>
N:	91
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Table 4: (Nos 1-63), Taurus faint sources survey sample Table 7: (Nos 64-91), Unresolved Taurus 60 mu.m sources
Ref:	=1992ApJ...386..248B
by	BEICHMAN C.A. , BOULANGER F., MOSHIR M.
	Astrophys. J., 386, 248-259 (1992)
	Star formation in Taurus. I. The IRAS faint source survey.
o	Tables 4, 7: <[BBM92] NN> (Nos 1-91)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBN91]
[BBN91]	(Batuski+Burns+Newberry+, 1991)
Write:	<<[BBN91] HHMMSS+DDMMSS>> <<[BBN91] JHHMMSS.ss+DDMMSS.s>> <<[BBN91] NN>>
N:	49+22+17
Object:	G in ClG (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Tables 1, 2: N=49+22 G in 30 ClG Table 3: N=14 G in the Sextans-Leo region, and N=3 in a field associated with ACO 2304. Objects have 2 formats 'JHHMMSS.ss+DDMMSS.s' and 'NN'
Ref:	=1991AJ....101.1983B
by	BATUSKI D.J. , BURNS J.O., NEWBERRY M.V., HILL J.M., DEEG H.-J., LAUBSCHER B.E., ELSTON R.J.
	Astron. J., 101, 1983-1996 (1991)
	Galaxy and cluster redshift observations in the Sextans-Leo region.
o	Tables 1, 2: <[BBN91] HHMMSS+DDMMSS> N=49+22. Table 3: <[BBN91] JHHMMSS.ss+DDMMSS.s> = <[BBN91] NN> (Nos 1-17).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBO2011]
[BBO2011]	(Bellazzini+Beccari+Oosterloo+, 2011)
Write:	<<[BBO2011] CN>>
N:	2
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	TNG DoLoRes spectroscopy and HST ACS photometry of N=2 clusters of stars in the dwarf galaxy VV 124.
in source:	VV 124 = UGC 4879
Ref:	=2011A&A...527A..58B
by	BELLAZZINI M. , BECCARI G., OOSTERLOO T.A., GALLETI S., SOLLIMA A., CORRENTI M., TESTA V., MAYER L., CIGNONI M., FRATERNALI F., GALLOZZI S.
	Astron. Astrophys., 527A, 58-58 (2011)
	An optical and HI study of the dwarf local group galaxy VV 124 = UGC 4879. A gas-poor dwarf with a stellar disk?
o	<[BBO2011] CN> (No. C1).
Ref:	=2011A&A...533A..37B
by	BELLAZZINI M. , PERINA S., GALLETI S., OOSTERLOO T.
	Astron. Astrophys., 533A, 37-37 (2011)
	HST-ACS photometry of the isolated dwarf galaxy VV124=UGC 4879. Detection of the blue horizontal branch and identification of two young star clusters.
o	Fig. 8, Table 4: <[BBO2011] CN> (No. C2) added. vv124: <[BPG2011b] NNNNN> N=69795 among (Nos 3-69872).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBP2005]
[BBP2005]	(Bykov+Bocchino+Pavlov, 2005)
Write:	<<[BBP2005] 11a>> <<[BBP2005] RN>> <<[BBP2005] JHHMMSS.ss+DDMMSS.s>>
N:	4
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observation of the source [BB2003] 11 in IC 443: the structure of the source is rather complex and looks like point sources: Nos 11a and 11b, a 3rd possible compact source 'J061803.39+222729.5', and an extended region of emission R1 in the NW part.
in source:	IC 443:[BB2003] 11 = [BB2003] 11
Ref:	=2005ApJ...624L..41B
by	BYKOV A.M. , BOCCHINO F., PAVLOV G.G.
	Astrophys. J., 624, 41-44 (2005)
	A hard extended X-ray source in the IC 443 supernova remnant resolved by Chandra: a fast ejecta fragment or a new pulsar wind nebula?
o	Fig.1, text: <[BBP2005] 11a> (Nos 11a-11b), <[BBP2005] RN> (No. R1), <[BBP2005] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBP2008]
[BBP2008]	(Beasley+Bridges+Peng+, 2008)= (AAT) = (HH)
Write:	<<[BBP2008] AATNNNNNN>> <<[BBP2008] HH-NNN>>
N:	134+44
Object:	GlCl + * + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	AAT 2dF spectroscopic observations of NGC 5128.
in source:	NGC 5128 = Cen A
Ref:	=2008MNRAS.386.1443B
by	BEASLEY M.A. , BRIDGES T., PENG E., HARRIS W.E., HARRIS G.L.H., FORBES D.A., MacKIE G.
	Mon. Not. R. Astron. Soc., 386, 1443-1463 (2008)
	A 2dF spectroscopic study of globular clusters in NGC 5128: probing the formation history of the nearest giant elliptical.
o	In Tables 2, 3, 4, the objects designated as HH-NNN are not [HHG2004] NNN, so we have created [BBP2008] HH-NNN for them.
o	Tables 2, 3, 4: <[BBP2008] AATNNNNNN> N=79+117+38, <[BBP2008] HH-NNN> N=44.
=E=	Catalogue in electronic form as J/MNRAS/386/1443
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBP95]
[BBP95]	(Bowen+Blades+Pettini, 1995)
Write:	<<[BBP95] HHMM+DDMM>>
N:	5
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	The authors use the letter 'G' for Galaxy, behind the format. Map for objects in Fig. 1, 8, 17. See also [BBP96], [BOB97]
Ref:	=1995ApJ...448..634B
by	BOWEN D.V. , BLADES J.C., PETTINI M.
	Astrophys. J., 448, 634-661 (1995)
	Interstellar Mg II absorption lines from low-redshift galaxies.
o	X-ray Seyfert ESO 141 = ESO 141-55, FCC 1100 misprint ? or = FCC B1100 ? (fig. 21)
o	Tables 1, 4, Fig. 8: <[BBP95] HHMM+DDMM> N=5
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBP96]
[BBP96]	(Bowen+Blades+Pettini, 1996)
Write:	<<[BBP96] HHMM+DDMM>> <<[BBP96] HHMM.m+DDMM>>
N:	5
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST FOS observations The authors use the letter 'G' for Galaxy, behind the format. See also [BBP95], [BOB97]
Ref:	=1996ApJ...464..141B
by	BOWEN D.V. , BLADES J.C., PETTINI M.
	Astrophys. J., 464, 141-157 (1996)
	Extended lyα-absorbing halos around nearby galaxies.
o	Tables 2, 5: <[BBP96] HHMM+DDMM>, <[BBP96] HHMM.m+DDMM> N=5
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBR2000]
[BBR2000]	(Brooks+Burton+Rathborne+, 2000)
Write:	<<[BBR2000] UN>>
N:	1
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=1 faint H2 emission clump labelled 'U1'. See also CO emission clumps [CB95].
in source:	NAME Keyhole Nebula
Ref:	=2000MNRAS.319...95B
by	BROOKS K.J. , BURTON M.G., RATHBORNE J.M., ASHLEY M.C.B., STOREY J.W.V.
	Mon. Not. R. Astron. Soc., 319, 95-102 (2000)
	Unlocking the Keyhole: H_{2} and PAH emission from molecular clumps in the Keyhole Nebula.
o	Table 2: <[BBR2000] U1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBR2002]
[BBR2002]	(Barrena+Biviano+Ramella+, 2002)
Write:	<<[BBR2002] NN>>
N:	78
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
in source:	ClG 0657-56
Ref:	=2002A&A...386..816B
by	BARRENA R. , BIVIANO A., RAMELLA M., FALCO E.E., SEITZ S.
	Astron. Astrophys., 386, 816-828 (2002)
	The dynamical status of the cluster of galaxies 1E 0657-56.
o	Table 1: <[BBR2002] NN> (Nos 1-78).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBR2015]
[BBR2015]	(Bacon+Brinchmann+Richard+, 2015)
Write:	<<[BBR2015] NNN>>
N:	586
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT MUSE spectroscopic observations of N=586 galaxies in the Hubble Deep Field South.
in source:	NAME HDF-S
Ref:	=2015A&A...575A..75B
by	BACON R. , BRINCHMANN J., RICHARD J., CONTINI T., DRAKE A., FRANX M., TACCHELLA S., VERNET J., WISOTZKI L., BLAIZOT J., BOUCHE N., BOUWENS R., CANTALUPO S., CAROLLO C.M., CARTON D., CARUANA J., CLEMENT B., DREIZLER S., EPINAT B., GUIDERDONI B., HERENZ C., HUSSER T.-O., KAMANN S., KERUTT J., KOLLATSCHNY W., KRAJNOVIC D., LILLY S., MARTINSSON T., MICHEL-DANSAC L., PATRICIO V., SCHAYE J., SHIRAZI M., SOTO K., SOUCAIL G., STEINMETZ M., URRUTIA T., WEILBACHER P., DE ZEEUW T.
	Astron. Astrophys., 575A, 75-75 (2015)
	The MUSE 3D view of the Hubble Deep Field South.
o	Table A.1: <[BBR2015] NNN> (Nos 0-585).
=E=	Catalogue in electronic form as J/A+A/575/A75
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBR99]
[BBR99]	(Benitez+Broadhurst+Rosati+, 1999) (Not yet in Simbad)
Write:	<<[BBR99] AA>>
N:	1
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Fig.9, Table 2: N=1 new faint object right and below the main arc.
in source:	AX J2019+112
Ref:	=1999ApJ...527...31B
by	BENITEZ N. , BROADHURST T., ROSATI P., COURBIN F., SQUIRES G., LIDMAN C., MAGAIN P.
	Astrophys. J., 527, 31-41 (1999)
	Deep imaging of AX J2019+112: the luminosity of a ``Dark cluster''.
o	Components A to D = [LSS84] 2016+112 A to D.
o	Fig.9, Table 2: <[BBR99] CA> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BBRCG
BBRCG	(Barsony+Burton+Russell+Carlstrom+Garden)
Write:	<<BBRCG NN>>
N:	61
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	NAME rho Oph Cloud
Ref:	=1989ApJ...346L..93B
by	BARSONY M. , BURTON M.G., RUSSELL A.P.G., CARLSTROM J.E., GARDEN R.
	Astrophys. J., 346, 93-96 (1989)
	Discovery of new 2 micron sources in ρ Ophiuchi.
o	<BBRCG NN> N=61
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BBRW
BBRW	(Balser+Bania+Rood+Wilson)
Write:	<<BBRW WNN(a)>> <<BBRW WNN(aN)>> <<BBRW G133.8(a)>> <<BBRW SNNN(a)>> <<BBRW SNNN(aN)>> <<BBRW SgrB2(aN)>> <<BBRW M17S(a)>>
N:	40
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=40 VLA components of 11 galactic HII regions.
in source:	W 3
in source:	GAL 133.8+01.4
in source:	SH 2-206
in source:	SH 2-209
in source:	NAME Sgr B2
in source:	NAME M 17S
in source:	W 43
in source:	W 49
in source:	W 51
in source:	SH 2-158
in source:	SH 2-162
Ref:	=1995ApJS..100..371B
by	BALSER D.S. , BANIA T.M., ROOD R.T., WILSON T.L.
	Astrophys. J., Suppl. Ser., 100, 371-388 (1995)
	The continuum structure of 11 galactic H II regions.
o	<BBRW WNN(aN)>, <BBRW G133.8(a)>, <BBRW SNNN(aN)>, <BBRW SgrB2(aN), <BBRW M17S(a)>, N=40.
Origin	of the Acronym: L (2001AJ....121..371B)
Details on Acronym: BBS
BBS	(Braun+Burton, Secondary clouds)
*****	Avoid the usage of BBS, prefer [SB2002]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBS2001]
[BBS2001]	(Bauer+Brandt+Sambruna+, 2001)
Write:	<<[BBS2001] CG X-N>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of the X-ray emission from the Circinus Galaxy (CG in the format). X-1 and X-2 are the 2 brightest off-nuclear sources among 16 CXOU sources.
in source:	NAME Circinus Galaxy
Ref:	=2001AJ....122..182B
by	BAUER F.E. , BRANDT W.N., SAMBRUNA R.M., CHARTAS G., GARMIRE G.P., KASPI S., NETZER H.
	Astron. J., 122, 182-193 (2001)
	A Chandra study of the Circinus galaxy point-source population.
o	Fig.1, Table 1: <[BBS2001] CG X-N> (Nos X-1, X-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBS2002]
[BBS2002]	(Balogh+Bower+Smail+, 2002)= (ba)
Write:	<<[BBS2002] Cl JHHMM NNN>> <<[BBS2002] Cl JHHMMa NNN>> <<[BBS2002] Cl JHHMMa/a NNN>>
N:	172
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 imaging and spectroscopy. N=317 galaxies in 9 clusters. In the format 'JHHMM' is the R.A. (J2000) of the ClG, the authors have not written the letter 'J'.
in source:	ClG J0818+5654
in source:	ClG J0819+7054
in source:	ClG J0841+7046
in source:	ClG J0849+3731
in source:	ClG J1309+3222
in source:	ClG J1444+6344
in source:	ClG J1633+5714
in source:	ClG J1701+6421
in source:	ClG J1702+6420
Ref:	=2002MNRAS.337..256B
by	BALOGH M. , BOWER R.G., SMAIL I., ZIEGLER B.L., DAVIES R.L., GAZTELU A., FRITZ A.
	Mon. Not. R. Astron. Soc., 337, 256-274 (2002)
	Galaxy properties in low X-ray luminosity clusters at z =0.25.
o	Table 4, Figs: <[BBS2002] Cl JHHMM NNN>, <[BBS2002] Cl JHHMMa NNN>, N=172.
=E=	Catalogue in electronic form as J/MNRAS/337/256
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBS2004]
[BBS2004]	(Bolton+Burles+Schlegel+, 2004)
Write:	<<[BBS2004] BG N.NNN>> <<[BBS2004] BG N.NNNN>>
N:	49+13+2+10+87
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	SDSS spectroscopic gravitational lens galaxies have a background (BG in the format) lensed galaxy defined by its redshift (N.NNNN in the format). When two galaxies have the same redshift, to the second is given z = (N.NNNN +0.0001) in the format. When galaxies have a redshift N.NNN, the format is N.NNN0. For the definitive full sample (N=131) see SLACS.
Ref:	=2004AJ....127.1860B
by	BOLTON A.S. , BURLES S., SCHLEGEL D.J., EISENSTEIN D.J., BRINKMANN J.
	Astron. J., 127, 1860-1882 (2004)
	Sloan Digital Sky Survey spectroscopic lens search. I. Discovery of intermediate-redshift star-forming galaxies behind foreground luminous red galaxies.
o	Table 1, col(7): <[BBS2004] BG N.NNNN> N=49.
Ref:	=2006ApJ...638..703B
by	BOLTON A.S. , BURLES S., KOOPMANS L.V.E., TREU T., MOUSTAKAS L.A.
	Astrophys. J., 638, 703-724 (2006)
	The Sloan Lens ACS Survey. I. A large spectroscopically selected sample of massive early-type lens galaxies.
o	Table 1, col(6): <[BBS2004] BG N.NNNN> N=13 added.
Ref:	=2006ApJ...640...62B
by	BOYCE E.R. , BOWMAN J.D., BOLTON A.S., HEWITT J.N., BURLES S.
	Astrophys. J., 640, 62-68 (2006)
	A search for radio gravitational lenses, using the Sloan Digital Sky Survey and the Very Large Array.
o	Table 1: SDSS J155030.75+521759.8 is a misprint for SDSS J155030.75+521705.0
o	Table 1, col(3): <[BBS2004] BG N.NNNN> N=2 added.
Ref:	=2007ApJ...667..176G
by	GAVAZZI R. , TREU T., RHODES J.D., KOOPMANS L.V.E., BOLTON A.S., BURLES S., MASSEY R.J., MOUSTAKAS L.A.
	Astrophys. J., 667, 176-190 (2007)
	The Sloan Lens ACS Survey. IV. The mass density profile of early-type galaxies out to 100 effective radii.
o	Table 1, col(zs): <[BBS2004] BG N.NNN> N=12 added.
Ref:	=2008ApJ...682..964B
by	BOLTON A.S. , BURLES S., KOOPMANS L.V.E., TREU T., GAVAZZI R., MOUSTAKAS L.A., WAYTH R., SCHLEGEL D.J.
	Astrophys. J., 682, 964-984 (2008)
	The Sloan lens ACS survey. V. The full ACS strong-lens sample.
o	Fig. 5, Table 4: <SLACS SDSS JHHMM+DDMM> N=131. Table 4: <SLACS SDSS JHHMM+DDMM source> N=131, <SLACS SDSS JHHMM+DDMM lens> N=131.
=E=	Catalogue in electronic form as J/ApJ/682/964
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBS2005]
[BBS2005]	(Bica+Bonatto+Santiago+, 2005)= ([BBS2005a]) = (W)
Write:	<<[BBS2005] W LLL.l+B.b>>
N:	2
Object:	* concentration (SIMBAD class: Region = Region defined in the Sky)
Stat:	is completely incorporated in Simbad
Note:	Search for the properties of two stellar concentrations in Centaurus, designated with a letter 'W' for Window in the sense of a case similar to Baade's window. Use of GSc and 2MASS archival data.
Ref:	=2005A&A...433..931B
by	BICA E. , BONATTO C., SANTIAGO B.X., KERBER L.O.
	Astron. Astrophys., 433, 931-940 (2005)
	A low-absorption disk zone at low Galactic latitude in Centaurus.
o	Text: <[BBS2005] W LLL.l+B.b> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBS2005a]
[BBS2005a]	(Bica+Bonatto+Santiago+, 2005)
*****	Avoid the usage of [BBS2005a], prefer [BBS2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBS2005b]
[BBS2005b]	(Blake+Bloom+Starr+, 2005) (Not yet in Simbad)
Write:	<<[BBS2005b] SN>>
N:	2
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Keck images revealed two sources within GRB 041219A field.
Ref:	=2005Natur.435..181B
by	BLAKE C.H. , BLOOM J.S., STARR D.L., FALCO E.E., SKRUTSKIE M., FENIMORE E.E., DUCHENE G., SZENTGYORGYI A., HORNSTEIN S., PROCHASKA J.X., McCABE C., GHEZ A., KONOPACKY Q., STAPELFELDT K., HURLEY K., CAMPBELL R., KASSIS M., CHAFFEE F., GEHRELS N., BARTHELMY S., CUMMINGS J.R., HULLINGER D., KRIMM H.A., MARKWARDT C.B., PALMER D., PARSONS A., McLEAN K., TUELLER J.
	Nature, 435, 181-184 (2005)
	An infrared flash contemporaneous with the γ-rays of GRB 041219a.
o	Text: <[BBS2005b] SN> (Nos S1-S2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBS2008]
[BBS2008]	(Bonatto+Bica+Santos, 2008)
Write:	<<[BBS2008] New Cluster N>>
N:	1
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Stat:	is completely incorporated in Simbad
Note:	Use of archival 2MASS data. Discovery of a new cluster in pair with PK 167-0.1.
Ref:	=2008MNRAS.386..324B
by	BONATTO C. , BICA E., SANTOS J.F.C.Jr
	Mon. Not. R. Astron. Soc., 386, 324-336 (2008)
	Discovery of an open cluster with a possible physical association with a planetary nebula.
o	Table 1: <[BBS2008] New Cluster N> (No. 1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBS2011]
[BBS2011]	(Bayo+Barrado+Stauffer+, 2011)
Write:	<<[BBS2011] C69-Sub-NNN>> <<[BBS2011] C69-IRAC-NNN>>
N:	5+10
Object:	* (SIMBAD class: Star)
Note:	N=5+10 candidate members of Collinder 69.
in source:	Cl Collinder 69
Ref:	=2011A&A...536A..63B
by	BAYO A. , BARRADO D., STAUFFER J., MORALES-CALDERON M., MELO C., HUELAMO N., BOUY H., STELZER B., TAMURA M., JAYAWARDHANA R.
	Astron. Astrophys., 536A, 63-63 (2011)
	Spectroscopy of very low mass stars and brown dwarfs in the λ Orionis star forming region. I. Enlarging the census down to the planetary mass domain in Collinder 69.
o	Table 6: <[BBS2011] C69-sub-NNN> (Nos 001-005), <[BBS2011] C69-IRAC-NNN> (Nos 001-010).
=E=	Catalogue in electronic form as J/A+A/536/A63
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBS2012]
[BBS2012]	(Brownstein+Bolton+Schlegel+, 2012)
Write:	<<[BBS2012] SDSS JHHMM+DDMM>> <<[BBS2012] SDSS JHHMM+DDMM source>>
N:	36*2
Object:	Poss. Grav. lens system (SIMBAD class: GravLensSystem_Candidate = Gravitational Lens System (lens+images) Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=25 definite and N=11 probable strong galaxy-galaxy gravitational lens systems from the BOSS Emission-Line Lens Survey (BELLS). See also [BBS2012].
Ref:	=2012ApJ...744...41B
by	BROWNSTEIN J.R. , BOLTON A.S., SCHLEGEL D.J., EISENSTEIN D.J., KOCHANEK C.S., CONNOLLY N., MARASTON C., PANDEY P., SEITZ S., WAKE D.A., WOOD-VASEY W.M., BRINKMANN J., SCHNEIDER D.P., WEAVER B.A.
	Astrophys. J., 744, 41 (2012)
	The BOSS Emission-Line Lens Survey (BELLS). I. A large spectroscopically selected sample of lens galaxies at redshift ~0.5.
o	Tables: <[BBS2012] SDSS JHHMM+DDMM> N=36, <[BBS2012] SDSS JHHMM+DDMM source> N=36.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBS98]
[BBS98]	(Bouwens+Broadhurst+Silk, 1998)
Write:	<<[BBS98] JHHMMSS.sss+DDMMSS.sss>>
N:	31
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
in source:	NAME HDFN
Ref:	=1998ApJ...506..557B
by	BOUWENS R. , BROADHURST T., SILK J.
	Astrophys. J., 506, 557-578 (1998)
	Cloning Hubble deep fields. I. A model-independent measurement of galaxy evolution.
o	Table 1: <[BBS98] JHHMMSS.sss+DDMMSS.sss> N=31.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBT2016]
[BBT2016]	(Bassa+Beswick+Tingay+, 2016)
Write:	<<[BBT2016] source N>>
N:	7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	MERLIN, VLBA, ATCA and Subaru observations of N=7 radio sources in the field of WISE J071634.59-190039.2.
in source:	WISE J071634.59-190039.2
Ref:	=2016MNRAS.463L..36B
by	BASSA C.G. , BESWICK R., TINGAY S.J., KEANE E.F., BHANDARI S., JOHNSTON S., TOTANI T., TOMINAGA N., YASUDA N., STAPPERS B.W., BARR E.D., KRAMER M., POSSENTI A.
	Mon. Not. R. Astron. Soc., 463L, 36-40 (2016)
	Optical and radio astrometry of the galaxy associated with FRB 150418.
o	Table 2: <[BBT2016] source N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBT95]
[BBT95]	(Belloni+Bruzual+Thimm+, 1995)
Write:	<<[BBT95] NNN>>
N:	107
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Tables 8, 9, and Fig. 2, 10: N=107 among (Nos 38-775)
in source:	GHO 093942+471306
Ref:	=1995A&A...297...61B
by	BELLONI P. , BRUZUAL G.A., THIMM G.J., ROESER H.-J.
	Astron. Astrophys., 297, 61-76 (1995)
	Detectability and incidence of E+A galaxies in the distant cluster Cl0939+472 (z=0.41).
o	Cl 0939+472 = [GHO86] 093942+471306
o	Tables 8, 9, Fig. 2, 10: <[BBT95] NNN> N=107 among (Nos 38-775)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBV2012]
[BBV2012]	(Bonafede+Bruggen+van Weeren+, 2012)
Write:	<<[BBV2012] MACSJHHMM.m+DDMM WW>> <<[BBV2012] MACSJHHMM.m+DDMM A>>
N:	4+14
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	GMRT 323MHz observations of N=4 relics and N=14 embedded radio sources in MACSJ1149.5+2223, MACSJ1752.0+4440 and MACSJ0553.4-3342
in source:	MCS J1149.0+2223
in source:	MCS J1752.0+4440
in source:	MCS J0553.0-3342
Ref:	=2012MNRAS.426...40B
by	BONAFEDE A. , BRUGGEN M., VAN WEEREN R., VAZZA F., GIOVANNINI G., EBELING H., EDGE A.C., HOEFT M., KLEIN U.
	Mon. Not. R. Astron. Soc., 426, 40-56 (2012)
	Discovery of radio haloes and double relics in distant MACS galaxy clusters: clues to the efficiency of particle acceleration.
o	Figs 1+5, Table 3: <[BBV2012] MACS JHHMM.m+DDMM WW> (Nos MACSJ1149.5+2223 W, MACSJ1149.5+2223 E, MACSJ1752.0+4440 NE, MACSJ1752.0+4440 SW). Figs 1+5+8, Table 4: <[BBV2012] MACSJHHMM.m+DDMM A> (Nos MACSJ1149.5+2223 A-G, MACSJ1752.0+4440 A-F, MACSJ0553.4-3342 A).
o	MACS J1752.040+44 and MACSJ1752.1+4440 are attributed to MCS J1752.0+4440 in Simbad.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BBW
BBW	(Bok+Bester+Wade)
Write:	<<BBW LLLBBa>>
N:	41
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Format based upon the galactic coordinates lI,bI of the object center. The first 3 digits are the whole-number part of the galactic longitude, the last 2 digits are the whole-number part of the galactic latitude. If the latitude is negative, the last 2 digits are italicized, that is not visible in SIMBAD, so BBW 30000 (+00) is BBW 30000a in SIMBAD, BBW 30000 (-00) is BBW 30000b in SIMBAD. Also published in: Daedalus, Proc. Am. Acad. Arts Sci. 86, 9-16.
Ref:	=1955HarRe.416....1B
by	BOK B.J. , BESTER M.J., WADE C.M.
	Harvard College Observatory - Reprints, 416, 1-16 (1955)
	Catalogue of H(II) regions in the Milky Way for longitudes 250°-355°.
o	BBW 30000 (+00) is BBW 30000a in SIMBAD, BBW 30000 (-00) is BBW 30000b in SIMBAD.
o	Table I: <BBW LLLBBa> N=41
Origin	of the Acronym: L (1974Ap&SS..27....3M)
Details on Acronym: BBW
BBW	(Brand+Blitz+Wouterloot)
*****	Avoid the usage of BBW, prefer Bran
Details on Acronym: [BBW2000]
[BBW2000]	(Brosch+Brook+Wisotzki+, 2000)
Write:	<<[BBW2000] AA NNNa>>
N:	777
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	FAUST observations of 4 fields: Dorado field: format 'FD NNN' Centaurus field: format 'FC NNN' M81 field: format 'FM NNN' Telescopium field: format 'FT NNN'. See also FAUST.
Ref:	=2000MNRAS.313..641B
by	BROSCH N. , BROOK A., WISOTZKI L., ALMOZNINO E., PRIALNIK D., BOWYER S., LAMPTON M.
	Mon. Not. R. Astron. Soc., 313, 641-655 (2000)
	FAUST observations in the Fourth Galactic Quadrant.
o	Table 2: <[BBW2000] FD NNNa>, <[BBW2000] FC NNNa>, <[BBW2000] FM NNNa>, <[BBW2000] FT NNNa>, N=733.
=E=	Catalogue in electronic form as J/MNRAS/313/641
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBW2011]
[BBW2011]	(Bagetakos+Brinks+Walter+, 2011)
Write:	<<[BBW2011] NGC NNNN NNN>> <<[BBW2011] Holmberg R NN>> <<[BBW2011] IC 2574 NN>> <<[BBW2011] DDO NNN N>>
N:	1046
Object:	HI Hole (SIMBAD class: HI = HI (21cm) Source)
Note:	N=1046 HI holes detected in 20 galaxies that are part of "The HI Nearby Galaxy Survey" (THINGS).
Ref:	=2011AJ....141...23B
by	BAGETAKOS I. , BRINKS E., WALTER F., DE BLOK W.J.G., USERO A., LEROY A.K., RICH J.W., KENNICUTT R.C.
	Astron. J., 141, 23 (2011)
	The fine-scale structure of the neutral interstellar medium in nearby galaxies.
o	Table 7: <[BBW2011] NGC NNNN NNN>, <[BBW2011] Holmberg R NN>, <[BBW2011] IC 2574 NN>, <[BBW2011] DDO NNN N>, N=1046.
=E=	Catalogue in electronic form as <J/AJ/141/23/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBW79]
[BBW79]	(Beichman+Becklin+Wynn-Williams, 1979)= (IRS) = (R)
Write:	<<[BBW79] Cep A N>> <<[BBW79] S 140 IRS Na>> <<[BBW79] S 140 IRS NW>> <<[BBW79] S 140 WW>> <<[BBW79] S 140 N>> <<[BBW79] S 255 IRS N>>
N:	16
Object:	(Rad) + (IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	N=3 radio-sources in Cep A MCld, format 'Cep A N', (Nos 1-3) sometimes found in the literature with a format 'R1 to R3' N=7 (IR) sources in Sh 2-140, format 'S 140 IRS N', (Nos 1-7), No. 3 is resolved in 3 point sources 3a to 3c, Nos 4 and 5 are also designated as [SFC83] VLA sources. and different (Nos 4-7) are created in 2002A&A...381..905W, designated as [WBP2002] in SIMBAD. N=2 radio-source in Sh 2-140, format 'S 140 WW' also designated as 'VLA NW' and 'VLA SE'. N=2 (IR) sources in Sh 2-255, format 'S 255 IRS N', (Nos 1-2), same as [HPF97] IRS 1 and 2.
in source:	NAME Cep A
in source:	SH 2-140
in source:	SH 2-255
Ref:	=1979ApJ...232L..47B
by	BEICHMAN C.A. , BECKLIN E.E., WYNN-WILLIAMS C.G.
	Astrophys. J., 232, 47-51 (1979)
	New multiple systems in molecular clouds.
o	Table 1: <[BBW79] Cep A N> (Nos 1-3), <[BBW79] S 140 IRS N> (Nos 1-3), <[BBW79] S 140 WW> (No. NW), <[BBW79] S 255 IRS N> (Nos 1-2).
Ref:	=1983ApJ...266..623S
by	SIMON M. , FELLI M., CASSAR L., FISCHER J., MASSI M.
	Astrophys. J., 266, 623-645 (1983)
	Infrared line and radio continuum emission of circumstellar ionized regions.
o	in ref list Simon et al 1981a is wrong
o	Table 2: <[SFC83] S140 N> (Nos 4-5) = <[BBW79] S140 IRS N> (Nos 4-5).
Ref:	=1989ApJ...338L..25S
by	SCHWARTZ P.R.
	Astrophys. J., 338, 25-28 (1989)
	Jets and bullets in S 140.
o	Table 1: <[BBW79] S 140 IRS NW> (Nos 2N and 2S) added.
Ref:	=1998ApJ...500..320Y
by	YAO Y. , ISHII M., NAGATA T., OGAWA Y., SATO S., WATANABE M., YAMASHITA T.
	Astrophys. J., 500, 320-328 (1998)
	Near-infrared polarimetric study of S140 IRS.
o	VLA 4 = [BBW79] S 140 IRS 4 = [SFC83] S140 4.
o	Fig.1: <[BBW79] S 140 WW> (No. SE).
Ref:	=2001ApJ...561..282K
by	KRAEMER K.E. , JACKSON J.M., DEUTSCH L.K., KASSIS M., HORA J.L., FAZIO G.G., HOFFMANN W.F., DAYAL A.
	Astrophys. J., 561, 282-298 (2001)
	Dust characteristics of massive star-forming sites in the mid-infrared.
o	Table 4: <KJD NN> (Nos 1-11). Text: <[BBW79] S140 IRS N> (Nos 6-7) added.
Ref:	=2001A&A...378..539P
by	PREIBISCH T. , BALEGA Y.Y., SCHERTL D., SMITH M.D., WEIGELT G.
	Astron. Astrophys., 378, 539-545 (2001)
	High-resolution near-infrared study of the deeply embedded young stellar object S140 IRS3.
o	Fig.1: <[BBW79] S 140 IRS 3a> (Nos 3a to 3c). Fig.1: <[PBS2001] A> (Nos A-F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BBWo
BBWo	(Brand+Blitz+Wouterloot)
*****	Avoid the usage of BBWo, prefer Bran
Origin	of the Acronym: L (2000PASP..112..542K)
Details on Acronym: [BBZ2012]
[BBZ2012]	(Bradley+Bouwens+Zitrin+, 2012)
Write:	<<[BBZ2012] A1703-zDNa>>
N:	7+2
Object:	Grav. lensed image of a G (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST ACS and WFC3 observations of z∼7 z850-dropout candidates in the field of the galaxy cluster A1703. Use of archival Spitzer IRAC data.
Ref:	=2012ApJ...747....3B
by	BRADLEY L.D. , BOUWENS R.J., ZITRIN A., SMIT R., COE D., FORD H.C., ZHENG W., ILLINGWORTH G.D., BENITEZ N., BROADHURST T.J.
	Astrophys. J., 747, 3 (2012)
	Through the looking glass: bright, highly magnified galaxy candidates at z ~ 7 behind A1703.
o	Fig. 2, Table 1: <[BBZ2012] A1703-zDNa> (Nos zD1-zD7, zD5a-zD5b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BBZ2014]
[BBZ2014]	(Bouwens+Bradley+Zitrin+, 2014)
Write:	<<[BBZ2014] MACSJHHMM-JD1>> <<[BBZ2014] JHHMMSS.ss+DDMMSS.s>> <<[BBZ2014] JHHMMSS.ss+DDMMSS.ss>>
N:	2+17+1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=18 candidate z∼8 galaxies in the CLASH fields.
Ref:	=2014ApJ...795..126B
by	BOUWENS R.J. , BRADLEY L., ZITRIN A., COE D., FRANX M., ZHENG W., SMIT R., HOST O., POSTMAN M., MOUSTAKAS L., LABBE I., CARRASCO M., MOLINO A., DONAHUE M., KELSON D.D., MENEGHETTI M., BENITEZ N., LEMZE D., UMETSU K., BROADHURST T., MOUSTAKAS J., ROSATI P., JOUVEL S., BARTELMANN M., FORD H., GRAVES G., GRILLO C., INFANTE L., JIMENEZ-TEJA Y., LAHAV O., MAOZ D., MEDEZINSKI E., MELCHIOR P., MERTEN J., NONINO M., OGAZ S., SEITZ S.
	Astrophys. J., 795, 126 (2014)
	A census of star-forming galaxies in the z ~ 9-10 universe based on HST+Spitzer observations over 19 CLASH clusters: three candidate z ~ 9-10 galaxies and improved constraints on the star formation rate density at z ~ 9.2.
o	Fig. 3, Table 2: <[BBZ2014] MACSJHHMM-JD1> (Nos MACSJ1115-JD1, MACSJ1720-JD1). Table 5: <[BBZ2014] JHHMMSS.ss+DDMMSS.s> N=17, <[BBZ2014] JHHMMSS.ss+DDMMSS.ss> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BC
BC	(Baldone obs., Carbon *)= (Baldone)
Write:	<<BC NNN>>
N:	318
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Ref:	=1974ISKZ....1....7A
by	ALKSNE Z.
	Issl. Solntsa Krasnykh Zvezd., 1, 7-22 (1974)
	Photographic photometry of carbon stars in the field with center on l=204.4°, b=-1.3°.
o	Table 1, col(1): <[A74] NN> (Nos 1-17). Table 1, col(2): <BC N> (Nos 1-9).
Ref:	=1974ISKZ....2....5A
by	ALKSNE Z. , OZOLINA V.
	Issl. Solntsa Krasnykh Zvezd., 2, 5-13 (1974)
	New carbon stars in galactic zones centered at l=90° and l=174°.
o	Identification charts
o	Table I: <BC NN> (Nos 10-33)
Ref:	=1974ISKZ....2...14D
by	DAUBE I. , OZOLINA V.
	Issl. Solntsa Krasnykh Zvezd., 2, 14-16 (1974)
	New carbon stars.
o	Table I: <BC NN> (Nos 34-39)
Ref:	=1975ISKZ....3...29A
by	ALKSNE Z. , OZOLINA V.
	Issl. Solntsa Krasnykh Zvezd., 3, 29-34 (1975)
	New carbon stars in the zones centered at galactic longitude l=86°.
o	Table I: <BC NN> (Nos 40-49)
Ref:	=1976ISKZ....4....5A
by	ALKSNE Z. , OZOLINA V.
	Issl. Solntsa Krasnykh Zvezd., 4, 5-11 (1976)
	New carbon stars in several fields.
o	Table I: <BC NN> (Nos 50-62)
Ref:	=1976ISKZ....5...15A
by	ALKSNIS A. , ALKSNE Z., OZOLINA V., EGLITIS I.
	Issl. Solntsa Krasnykh Zvezd., 5, 15-22 (1976)
	New carbon stars in the zones centered at the galactic longitudes l=94 °. and l=178°.
o	Table I: <BC NN> (Nos 63-77)
Ref:	=1977ISKZ....6...55A
by	ALKSNIS A. , ALKSNE Z., OZOLINA V.
	Issl. Solntsa Krasnykh Zvezd., 6, 55-67 (1977)
	New carbon stars in the zone of galactic latitude b=-7°.
o	Table I: <BC NNN> (Nos 78-109)
Ref:	=1978ISKZ....8....5A
by	ALKSNIS A. , ALKSNE Z., OZOLINA V., PLATAIS I.
	Issl. Solntsa Krasnykh Zvezd., 8, 5-25 (1978)
	New carbon stars in the zone centered at the galactic latitude b=+7°.
o	Identification charts
o	Table I: <BC NNN> (Nos 110-184)
Ref:	=1979ISKZ...10...23P
by	PLATAIS I.
	Issl. Solntsa Krasnykh Zvezd., 10, 23-32 (1979)
	Observations of the new carbon star BC 185.
o	<BC 185>. Table 1: <[P79] NN> (Nos 1-12). Table 2: <[P79] A> (Nos A-G).
Ref:	=1979ATsir1042....6P
by	PLATAIS I.
	Astron. Tsirk., 1042, 6-8 (1979)
	New carbon stars in several fields.
o	<BC NNN> (Nos 186-200)
Ref:	=1981ISKZ...12...24A
by	ALKSNE Z. , ALKSNIS A.
	Issl. Solntsa Krasnykh Zvezd., 12, 24-30 (1981)
	17 new carbon stars BC 201 - BC 217.
o	<BC NNN> (Nos 201-217).
Ref:	=1981ISKZ...13....5A
by	ALKSNE A. , ALKSNIS A., EGLITIS I.
	Issl. Solntsa Krasnykh Zvezd., 13, 5-11 (1981)
	New carbon stars at the galactic longitudes 128-140.
o	<BC NNN> (Nos 218-234)
Ref:	=1983NInfo..52..138A
by	ALKSNE A. , ALKSNIS A., EGLITIS I.
	Naucnye Informacii, 52, 138-None (1983)
	Carbon stars found on infrared plates at the galactic longitude 86.
o	<BC NNN> (Nos 235-245)
Ref:	=1983ISKZ...19...40A
by	ALKSNIS A. , OZOLINA V.
	Issl. Solntsa Krasnykh Zvezd., 19, 40-46 (1983)
	Search for faint carbon stars in field centered l=86, b=0.
o	Table 2: <BC NNN> (Nos 246-255)
Ref:	=1987ISKZ...25....5A
by	ALKSNIS A. , ALKSNE Z., PLATAIS I., OZOLINA V.
	Issl. Solntsa Krasnykh Zvezd., 25, 5-12 (1987)
	New carbon stars at galactic longitude 82°.
o	Table II: <BC NN> (Nos 256-272)
Ref:	=1988NInfo..65..162A
by	ALKSNIS A. , ALKSNE Z., OZOLINA V., PLATAIS I.
	Naucnye Informacii, 65, 162-173 (1988)
	New carbon stars BC 273 - BC 310 found at the galactic longitude l = 94°.
o	Table 2: <BC NNN> (Nos 273-310)
Ref:	=1988ISKZ...29...16A
by	ALKSNIS A. , ALKSNE Z., PLATAIS I., OZOLINA V.
	Issl. Solntsa Krasnykh Zvezd., 29, 16-21 (1988)
	New carbon stars BC 311 - BC 318.
o	Table 2: <BC NNN> (Nos 311-318)
=E=	Catalogue in electronic form as III/140
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BC2002]
[BC2002]	(Berghofer+Christian, 2002)
Write:	<<[BC2002] NNN>>
N:	138
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC and HRI observations of NGC 2244.
in source:	NGC 2244
Ref:	=2002A&A...384..890B
by	BERGHOEFER T.W. , CHRISTIAN D.J.
	Astron. Astrophys., 384, 890-898 (2002)
	Optical properties of X-ray selected stars in NGC 2244 in the Rosette Nebula.
o	Table 3: <[BC2002] NNN> (Nos 1-138).
=E=	Catalogue in electronic form as J/A+A/384/890
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BC2009]
[BC2009]	(Barton+Cooke, 2009)
Write:	<<[BC2009] JHHMMSS.ss+DDMMSS.s>>
N:	20
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck I LRIS-B spectroscopy of N=20 galaxies in the field of QSOs.
Ref:	=2009AJ....138.1817B
by	BARTON E.J. , COOKE J.
	Astron. J., 138, 1817-1829 (2009)
	Mg II absorption characteristics of a volume-limited sample of galaxies at z ~ 0.1.
o	Table 1, col(2): <[BC2009] JHHMMSS.ss+DDMMSS.s> N=20.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BC2010]
[BC2010]	(Bibby+Crowther, 2010)
Write:	<<[BC2010] NNa>> <<[BC2010] GHR NN>> <<[BC2010] GHR A>>
N:	99+15+4
Object:	Em. Obj. + HII (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS1 imaging and spectroscopic survey of NGC 7793.
in source:	NGC 7793
Ref:	=2010MNRAS.405.2737B
by	BIBBY J.L. , CROWTHER P.A.
	Mon. Not. R. Astron. Soc., 405, 2737-2753 (2010)
	A Very Large Telescope imaging and spectroscopic survey of the Wolf-Rayet population in NGC7793.
o	Table 2: <[BC2010] NNa> N=99 among (Nos 1-74b). Table 7: <[BC2010] GHR NN> (Nos 1-15), <[BC2010] GHR A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BC2012]
[BC2012]	(Bibby+Crowther, 2012)
Write:	<<[BC2012] NNN>> <<[BC2012] HN>> <<[BC2012] HII NN>>
N:	160+4+29
Object:	Poss. WR + HII (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT FORS1 observations of N=160 candidate Wolf-Rayet sources and N=4+29 HII regions in NGC 5068.
in source:	NGC 5068
Ref:	=2012MNRAS.420.3091B
by	BIBBY J.L. , CROWTHER P.A.
	Mon. Not. R. Astron. Soc., 420, 3091-3107 (2012)
	The Wolf-Rayet population of the nearby barred spiral galaxy NGC 5068 uncovered by the Very Large Telescope and Gemini.
o	Table 2: <[BC2012] NNN> (Nos 1-160), <[BC2012] HN> (Nos H1-H4). Table 6: <[BC2012] HII NN> N=29 among (Nos 1-32).
=E=	Catalogue in electronic form as J/MNRAS/420/3091
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BC71]
[BC71]	(Bertola+Ciatti, 1971) (Not yet in Simbad)
Write:	<<[BC71] NGC 3811 a>>
N:	7
Object:	* (SIMBAD class: Star)
Note:	N=7 reference stars in the field of NGC 3811, host of SN 1969C
Ref:	=1971MmSAI..42...67B
by	BERTOLA F. , CIATTI F.
	Mem. Soc. Astron. Ital., 42, 67-72 (1971)
	Spectrum and light curve of the supernova in NGC 3811.
o	Table II, Fig.2: <[BC71] NGC 3811 a> (Nos a-g).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BC86]
[BC86]	(Barbieri+Cristiani, 1986)= ([BC86a])
Write:	<<[BC86] HHMM+DDMMA>>
N:	208
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Ref:	=1986A&AS...63....1B
by	BARBIERI C. , CRISTIANI S.
	Astron. Astrophys., Suppl. Ser., 63, 1-26 (1986)
	Quasar candidates in the field of SA 94 (2h53m,+0 20').
o	<[BC86] HHMM+DDMMA> N=208
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BC86a]
[BC86a]	(Barbieri+Cristiani, 1986)
*****	Avoid the usage of [BC86a], prefer [BC86]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BC86b]
[BC86b]	(Bachiller+Cernicharo, 1986)= (IRS)
Write:	<<[BC86b] LDN 1448 IRS NA>> <<[BC86b] LDN 1455 IRS N>>
N:	3+6+4
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	LDN 1448
in source:	LDN 1455
Ref:	=1986A&A...168..262B
by	BACHILLER R. , CERNICHARO J.
	Astron. Astrophys., 168, 262-270 (1986)
	Physical and chemical conditions in Perseus globules from NH3 and HC3N observations.
o	Fig 1: <[BC86b] LDN 1448 IRS N> (Nos 1-3). Fig 2: <[BC86b] LDN 1455 IRS N> (Nos 1-3).
Ref:	=2000ApJ...529..477L
by	LOONEY L.W. , MUNDY L.G., WELCH W.J.
	Astrophys. J., 529, 477-498 (2000)
	Unveiling the circumstellar envelope and disk: a subarcsecond survey of circumstellar structures.
o	Table 3, Fig.7b: <[BC86b] LDN 1448 IRS NA> (Nos 3A-3C). Table 3, Fig.10b: <[SVS76] NGC 1333 NNAN> (Nos 13A-13C, 13A1-13A2). Table 3, Fig. 15: <[LMW2000] VLA 1623A> (Nos A-B).
Ref:	=2006ApJ...645.1246J
by	JORGENSEN J.K. , HARVEY P.M., EVANS II N.J., HUARD T.L., ALLEN L.E., PORRAS A., BLAKE G.A., BOURKE T.L., CHAPMAN N., CIEZA L., KOERNER D.W., LAI S.-P., MUNDY L.G., MYERS P.C., PADGETT D.L., REBULL L., SARGENT A.I., SPIESMAN W., STAPELFELDT K.R., VAN DISHOECK E.F., WAHHAJ Z., YOUNG K.E.
	Astrophys. J., 645, 1246-1263 (2006)
	The Spitzer c2d survey of large, nearby, interstellar clouds. III. Perseus observed with IRAC.
o	Fig.14: <[BC86b] LDN 1455 IRS N> (Nos 4-6) added. Table 5: <[JHE2006] L1448-C(W)> (Nos C(N), C(S)). Paragr. 6.1, 6.2: <[JHE2006] JHHMMSS+DDMMSS> N=4.
Ref:	=2007ApJ...656..293J
by	JORGENSEN J.K. , JOHNSTONE D., KIRK H., MYERS P.C.
	Astrophys. J., 656, 293-305 (2007)
	Current star formation in the Perseus molecular cloud: constraints from unbiased submillimeter and mid-infrared surveys.
o	Table 3: <[JJK2007] NN> (Nos 1-49). Table 3: <[BC86b] LDN 1455 IRS N> (No. 4) added.
Ref:	=2007ApJ...659.1404T
by	TOBIN J.J. , LOONEY L.W., MUNDY L.G., KWON W., HAMIDOUCHE M.
	Astrophys. J., 659, 1404-1419 (2007)
	Imaging scattered light from the youngest protostars in L 1448: signatures of outflows.
o	Paragr. 4.1: <[BC86b] LDN 1448 IRS NA> (Nos 2A-2B) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BC86c]
[BC86c]	(Bieging+Crutcher, 1986)
Write:	<<[BC86c] A>> <<[BC86c] A'>>
N:	13+1
Object:	OH Cloud (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	VLA observations toward Cas A. N=14 OH clouds are observed.
in source:	NAME Cas A
Ref:	=1986ApJ...310..853B
by	BIEGING J.H. , CRUTCHER R.M.
	Astrophys. J., 310, 853-871 (1986)
	VLA observations of 1667 MHz OH absorption toward Cassiopeia A.
o	Table 1: <[BC86c] A> (Nos A-M), <[BC86c] A'> (No. C').
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BC94]
[BC94]	(Boyce+Cohen, 1994)
Write:	<<[BC94] Clump N>> <<[BC94] Filament A>> <<[BC94] Spur R>>
N:	7+6+5
Object:	Clump + Filament + Spur (SIMBAD class: Radio = Radio Source)
in source:	NAME Gal Center
Ref:	=1994A&AS..107..563B
by	BOYCE P.J. , COHEN R.J.
	Astron. Astrophys., Suppl. Ser., 107, 563-647 (1994)
	A large-scale survey of OH in the galactic centre.
o	Table 1: <[BC94] Clump N> N=7. Table 2: <[BC94] Filament A> N=6. Table 3: <[BC94] Spur R> N=5
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BC98]
[BC98]	(Buote+Canizares, 1998)
Write:	<<[BC98] N>> <<[BC98] WWa>>
N:	8+2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	From ROSAT PSPC and HRI archives
in source:	NGC 3923
Ref:	=1998MNRAS.298..811B
by	BUOTE D.A. , CANIZARES C.R.
	Mon. Not. R. Astron. Soc., 298, 811-823 (1998)
	X-ray isophote shapes and the mass of NGC 3923.
o	Table 1: <[BC98] N> (Nos 1-8), <[BC98] WWa> (Nos NWa-NWb).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCA2007]
[BCA2007]	(Bertoldi+Carilli+Aravena+, 2007)= (VLA)
Write:	<<[BCA2007] VLA JHHMMSS.ss+DDMMSS.s>>
N:	30
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA 1.4GHz counterpart of COSMOSMAMBO mm sources in the COSMOS field.
in source:	NAME COSMOS Field
Ref:	=2007ApJS..172..132B
by	BERTOLDI F. , CARILLI C., ARAVENA M., SCHINNERER E., VOSS H., SMOLCIC V., JAHNKE K., SCOVILLE N., BLAIN A., MENTEN K.M., LUTZ D., BRUSA M., TANIGUCHI Y., CAPAK P., MOBASHER B., LILLY S., THOMPSON D., AUSSEL H., KREYSA E., HASINGER G., AGUIRRE J., SCHLAERTH J., KOEKEMOER A.
	Astrophys. J., Suppl. Ser., 172, 132-149 (2007)
	COSBO: the MAMBO 1.2 millimeter imaging survey of the COSMOS field.
o	Objects refered as COSMOS 1211238, 1211239, 1240610, 1252837, 1252838, 1259096, 1605942, 1654929, 1654930, 1950977, 1958423, in Table 2 do not exist in the public COSMOS catalogue 2007ApJS..172...99C and have not been created in Simbad.
o	Tables 1,2 col(1): <COSMOSMAMBO NNWN> N=27 among (Nos 1-37) +19 +2. Table 1, col(2): <COSMOSMAMBO MM JHHMMSS+DDMMSS> N=27. Table 1, col(VLA): <[BCA2007] VLA JHHMMSS.ss+DDMMSS.s> N=30.
=E=	Catalogue in electronic form as <II/284/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCB2001]
[BCB2001]	(Barger+Cowie+Bautz+, 2001)
Write:	<<[BCB2001] ACO 370 NN>> <<[BCB2001] ACO 370 SNN>> <<[BCB2001] CDFN NN>>
N:	15+14+34
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra hard X-ray sources in ACO 370 and the CDFN.
in source:	ACO 370
in source:	NAME CDFN
Ref:	=2001AJ....122.2177B
by	BARGER A.J. , COWIE L.L., BAUTZ M.W., BRANDT W.N., GARMIRE G.P., HORNSCHEMEIER A.E., IVISON R.J., OWEN F.N.
	Astron. J., 122, 2177-2189 (2001)
	Supermassive black hole accretion history inferred from a large sample of Chandra hard X-ray sources.
o	Fig.1, Table 1: <[BCB2001] ACO 370 NN> (Nos 0-14). Table 2: <[BCB2001] ACO 370 SNN> (Nos S0-S13). Table 3: <[BCB2001] CDFN NN> (Nos 0-33).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCB89]
[BCB89]	(Barnes+Crutcher+Bieging+, 1989)= BCBSW = (IRS)
Write:	<<[BCB89] IRS NNa>>
N:	31+1
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	IRS 1 and IRS 2 where already existing, respectively discovered in 1968PASP...80...20G and 1974ApJ...193..373G, and also designated in SIMBAD as NGC 2024 1 and 2. IRS 2b is discovered later as the candidate ionizing star of NGC 2024.
in source:	NGC 2024
Ref:	=1989ApJ...342..883B
by	BARNES P.J. , CRUTCHER R.M., BIEGING J.H., STOREY J.W.V., WILLNER S.P.
	Astrophys. J., 342, 883-907 (1989)
	Orion B (NGC 2024). I. VLA and IR observations of the HII region.
o	Table 1: <[BCB89] IRS NN> (Nos 1-31)
Ref:	=2003A&A...404..249B
by	BIK A. , LENORZER A., KAPER L., COMERON F., WATERS L.B.F.M., DE KOTER A., HANSON M.M.
	Astron. Astrophys., 404, 249-254 (2003)
	Identification of the ionizing source of NGC 2024.
o	Fig. 1 : IRS N = [BCB89] IRS N. G206.543-16.347 = [KCW94] 206.543-16.347
o	<[BCB89] IRS NNa> (No. 2b) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCB99]
[BCB99]	(Buta+Crocker+Byrd, 1999)
Write:	<<[BCB99] NNN>>
N:	780
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST WFPC2 observations of the galaxy ESO 565-11. Table 1: N=780 among 783 Cl*, among which N=21 are stars (Table 2).
in source:	ESO 565-11
Ref:	=1999AJ....118.2071B
by	BUTA R. , CROCKER D.A., BYRD G.G.
	Astron. J., 118, 2071-2100 (1999)
	A Hubble Space Telescope optical and ground-based near-infrared study of the giant nuclear ring in ESO 565-11.
o	Table 1: <[BCB99] NNN> N=780 among (Nos 1-783).
=E=	Catalogue in electronic form as J/AJ/118/2071
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BCBSW
BCBSW	(Barnes+Crutcher+Bieging+Storey+Willner)
====>	Equivalent to: [BCB89]
Origin	of the Acronym: L (1995A&A...296L..21F)
Details on Acronym: [BCC2001]
[BCC2001]	(Bond+Churchill+Charlton+, 2001) (Not yet in Simbad)
Write:	<<[BCC2001] NN>>
N:	13
Object:	Cloud (SIMBAD class: Cloud)
Note:	N=13 clouds in MC3 1331+17.0 field.
Ref:	=2001ApJ...557..761B
by	BOND N.A. , CHURCHILL C.W., CHARLTON J.C., VOGT S.S.
	Astrophys. J., 557, 761-769 (2001)
	Evidence for expanding superbubbles in a galaxy at z=0.7443.
o	Galaxy in tittle = [LBB97] MC 1331+170 5.
o	Table 1: <[BCC2001] NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCC2003]
[BCC2003]	(Bertoldi+Carilli+Cox+, 2003)= [BCC2003a]
Write:	<<[BCC2003] J1148+5251 mm-WW>>
N:	3
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	IRAM 30m telescope observations. N=3 mm field sources in the direction of QSO SDSS J114816.64+525150.3, with in the format, a direction given from the QSO.
Ref:	=2003A&A...406L..55B
by	BERTOLDI F. , CARILLI C.L., COX P., FAN X., STRAUSS M.A., BEELEN A., OMONT A., ZYLKA R.
	Astron. Astrophys., 406, 55-58 (2003)
	Dust emission from the most distant quasars.
o	Table 1: FIRST-SW and FIRST-NE = FIRST J114812.1+525107 and FIRST J114819.5+525212 respectively in SIMBAD.
o	Table 1: <[BCC2003] J1148+5251 mm-WW> (Nos SW, NE, E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCC2003a]
[BCC2003a]	(Bertoldi+Carilli+Cox+, 2003)
*****	Avoid the usage of [BCC2003a], prefer [BCC2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCC2003b]
[BCC2003b]	(Barcons+Carballo+Carrera+, 2003)
Write:	<<[BCC2003b] Source N>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of RX J1011.2+5545 field. Source 1 is the RX counterpart, source 2 is a fainter X-ray source. See also [BCC98].
Ref:	=2003MNRAS.343..137B
by	BARCONS X. , CARBALLO R., CARRERA F.J., CEBALLOS M.T., GONZALEZ-SERRANO J.I., PAREDES J.M., RIBO M., WARWICK R.S.
	Mon. Not. R. Astron. Soc., 343, 137-142 (2003)
	On the origin of the X-ray emission from a narrow-line radio quasar at z > 1.
o	p. 140, 7C 434 = 7C 1007+5559
o	Text: <[BCC2003b] Source N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCC2014]
[BCC2014]	(Barger+Cowie+Chen+, 2014)
Write:	<<[BCC2014] CDFN NN>>
N:	49
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	15m James Clerk Maxwell Telescope SCUBA-2 spectroscopic observations of N=49 sources in a field containing the GOODS North Field.
in source:	NAME GOODS North Field
Ref:	=2014ApJ...784....9B
by	BARGER A.J. , COWIE L.L., CHEN C.-C., OWEN F.N., WANG W.-H., CASEY C.M., LEE N., SANDERS D.B., WILLIAMS J.P.
	Astrophys. J., 784, 9 (2014)
	Is there a maximum star formation rate in high-redshift galaxies?
o	Table 1: <[BCC2014] CDFN NN> (Nos 1-49).
=E=	Catalogue in electronic form as <J/ApJ/784/9/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCC85]
[BCC85]	(Bajaja+Cappa De Nicolau+Cersosimo+, 1985)
Write:	<<[BCC85] NNN>>
N:	742
Object:	HVC (SIMBAD class: HVCld = High-velocity Cloud)
Note:	Maps Figs2-4
Ref:	=1985ApJS...58..143B
by	BAJAJA E. , CAPPA DE NICOLAU C.E., CERSOSIMO J.C., LOISEAU N., MARTIN M.C., MORRAS R., OLANO C.A., POPPEL W.G.L.
	Astrophys. J., Suppl. Ser., 58, 143-165 (1985)
	A new general survey of high-velocity neutral hydrogen in the southern hemisphere.
o	Table 1: <[BCC85] NNN> (Nos 1-742)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCC97]
[BCC97]	(Bower+Castander+Couch+, 1997)
Write:	<<[BCC97] ANNNN.NNAA ANNA>>
N:	187
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	N=187 galaxies in 7 CEMM clusters. Maps in Figures 1.
in source:	CEMM F1557.19TC
in source:	CEMM F1652.20CR
in source:	CEMM F1637.23TL
in source:	CEMM J2175.15TR
in source:	CEMM J2175.23C
in source:	CEMM F1835.22CR
in source:	CEMM F1835.2CL
Ref:	=1997MNRAS.291..353B
by	BOWER R.G. , CASTANDER F.J., COUCH W.J., ELLIS R.S., BOHRINGER H.
	Mon. Not. R. Astron. Soc., 291, 353-371 (1997)
	A dynamical study of optically selected distant clusters.
o	Clusters with a format 'ANNNN.NNAA' are CEMM in SIMBAD
o	Table 2, Fig.1: <[BCC97] ANNNN.NNAA ANNA> N=187
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCC98]
[BCC98]	(Barcons+Carballo+Ceballos+, 1998)
Write:	<<[BCC98] JHHMMSS.s+DDMMSS>>
N:	1
Object:	AGN (SIMBAD class: AGN = Active Galaxy Nucleus)
Stat:	is completely incorporated in Simbad
Note:	The multi-wavelength study of the source RX J1011.2+5545 discovered in a ROSAT observation shows that it is an obscured high redshift radio-loud AGN. See also [BCC2003b].
Ref:	=1998MNRAS.301L..25B
by	BARCONS X. , CARBALLO R., CEBALLOS M.T., WARWICK R.S., GONZALEZ-SERRANO J.I.
	Mon. Not. R. Astron. Soc., 301, 25-29 (1998)
	Discovery of an X-ray-selected radio-loud obscured AGN at z = 1.246.
o	Text: <[BCC98] JHHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCC99]
[BCC99]	(Buonanno+Corsi+Castellani+, 1999) (Not yet in Simbad)
Write:	<<[BCC99] WFN NNNN>>
N:	11788
Object:	* in Cl* (SIMBAD class: Star)
Note:	The authors use observations from the HST, with a Wide Field (WF in the format) camera, for the fields 2, 3, 4, in Fornax 4 cluster.
in source:	NAME Fornax 4
Ref:	=1999AJ....118.1671B
by	BUONANNO R. , CORSI C.E., CASTELLANI M., MARCONI G., FUSI PECCI F., ZINN R.
	Astron. J., 118, 1671-1683 (1999)
	Hubble space telescope photometry of the Fornax dwarf spheroidal galaxy: cluster 4 and its field.
o	Table 1: <[BCC99] WF2 NNNN> (Nos 1-4059), <[BCC99] WF3 NNNN> (Nos 1-4202), <[BCC99] WF4 NNNN> (Nos 1-3527).
=E=	Catalogue in electronic form as J/AJ/118/1671
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BCD
BCD	(Bica+Claria+Dottori)
Write:	<<NAME BCD N>>
N:	1
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1992AJ....103.1859B
by	BICA E. , CLARIA J.J., DOTTORI H.
	Astron. J., 103, 1859-1871 (1992)
	Bar star clusters in the LMC: formation history from UBV integrated photometry.
o	<NAME BCD 1> = ANON 0521.7-6927
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BCD2000]
[BCD2000]	(Blum+Conti+Damineli, 2000)
Write:	<<[BCD2000] W42 N>>
N:	3
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=3 brightest stars in W 42 Cluster. See also [BDC99], [BDC2001], FBDDC
in source:	NAME W 42 Cluster
Ref:	=2000AJ....119.1860B
by	BLUM R.D. , CONTI P.S., DAMINELI A.
	Astron. J., 119, 1860-1871 (2000)
	The stellar content of obscured galactic giant H II regions. II. W42.
o	Par. 2.1 : standard 9170 is GSPC S875-C, 9172 is GSPC S279-F.
o	Fig.1a: <[BCD2000] W42 N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCD2004]
[BCD2004]	(Borys+Chapman+Donahue+, 2004)
Write:	<<[BCD2004] ARCN>> <<[BCD2004] ARC1 ci>> <<[BCD2004] A>> <<[BCD2004] AN>>
N:	2+1+2+6+1
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Stat:	is completely incorporated in Simbad
Note:	New SCUBA image of the cluster 1E 0451.6-0305. N=2 arcs, ARC1 and ARC2, already observed as [LGH99] MS 0451.6-0305 A1 and A2, and one counterimage (ci in the format of ARC1). N=2 sources B and C, a pair of EROs re-imaged in 3 places: B1 to B3, C1 to C3. N=1 smm blue galaxy P. See also [BGK2007].
in source:	1E 0451.6-0305 = ClG 0451-0305
Ref:	=2004MNRAS.352..759B
by	BORYS C. , CHAPMAN S., DONAHUE M., FAHLMAN G., HALPERN M., KNEIB J.-P., NEWBURY P., SCOTT D., SMITH G.P.
	Mon. Not. R. Astron. Soc., 352, 759-767 (2004)
	The nature of a gravitationally lensed submillimetre arc in MS0451.6-0305: two interacting galaxies at z~ 2.9?
o	Figs 2, 4, Table 1: <[BCD2004] ARCN> (Nos ARC1, ARC2), <[BCD2004] ARC1 ci> N=1, <[BCD2004] A> (Nos B, C, P), <[BCD2004] AN> (Nos B1-B3, C1-C3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCD2005]
[BCD2005]	(Brusa+Comastri+Daddi+, 2005)
Write:	<<[BCD2005] NNN>>
N:	97
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton observations of X-ray sources identified as Extremely Red Objects.
Ref:	=2005A&A...432...69B
by	BRUSA M. , COMASTRI A., DADDI E., POZZETTI L., ZAMORANI G., VIGNALI C., CIMATTI A., FIORE F., MIGNOLI M., CILIEGI P., ROETTGERING H.J.A.
	Astron. Astrophys., 432, 69-81 (2005)
	XMM-Newton observations of Extremely Red Objects and the link with luminous, X-ray obscured quasars.
o	Tables 1, 2: <[BCD2005] NNN> N=97 among (Nos 61-367).
=E=	Catalogue in electronic form as J/A+A/432/69
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCD2008]
[BCD2008]	(Butt+Combi+Drake+, 2008)
Write:	<<[BCD2008] A>> <<[BCD2008] XN>>
N:	9+2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra X-ray observations of the field around TeV J2032+4130.
Ref:	=2008MNRAS.385.1764B
by	BUTT Y.M. , COMBI J.A., DRAKE J., FINLEY J.P., KONOPELKO A., LISTER M., RODRIGUEZ J., SHEPHERD D.
	Mon. Not. R. Astron. Soc., 385, 1764-1770 (2008)
	TeV J2032+4130: a not-so-dark accelerator ?
o	In Chap 3 : TeV J2032+4131 is a misprint for TeV J2032+4130.
o	Fig.1, Table 2: <[BCD2008] A> (Nos A-I). Fig.1, Table 2: <[BCD2008] XN> (Nos X1-X2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCD2014]
[BCD2014]	(Blair+Chandar+Dopita+, 2014)
Write:	<<[BCD2014] NN>>
N:	63
Object:	SNR (SIMBAD class: SNRemnant = SuperNova Remnant)
Stat:	is completely incorporated in Simbad
Note:	HST WFC3 observations of N=63 SNRs in M83.
in source:	M 83 = NGC 5236
Ref:	=2014ApJ...788...55B
by	BLAIR W.P. , CHANDAR R., DOPITA M.A., GHAVAMIAN P., HAMMER D., KUNTZ K.D., LONG K.S., SORIA R., WHITMORE B.C., WINKLER P.F.
	Astrophys. J., 788, 55 (2014)
	An expanded HST/WFC3 survey of M83: project overview and targeted supernova remnant search.
o	Tables 3-4: <[BCD2014] NN> (Nos 1-63).
=E=	Catalogue in electronic form as J/ApJ/788/55
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCD2018]
[BCD2018]	(Baratella+Carraro+D'orazi+, 2018)
Write:	<<[BCD2018] NNNN>>
N:	7
Object:	* (SIMBAD class: Star)
Note:	Special Astrophysical Observatory 6-m BTA telescope spectroscopic observations of N=7 candidate red giant stars in the Tombaugh 5 open cluster.
in source:	Cl Tombaugh 5
Ref:	=2018AJ....156..244B
by	BARATELLA M. , CARRARO G., D'ORAZI V., SEMENKO E.A.
	Astron. J., 156, 244-244 (2018)
	Radial velocity and chemical composition of evolved stars in the open clusters NGC 6940 and Tombaugh 5.
o	Table 1: <[BCD2018] NNNN> N=7 among (Nos 6-8099).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCD86]
[BCD86]	(Baart+Cohen+Davies+, 1986) (Not yet in Simbad)
Write:	<<[BCD86] Maser A>> <<[BCD86] Cluster N>>
N:	15+4
Object:	Maser (SIMBAD class: Maser)
Note:	Table 1: N=15 OH masers in W75N, (Nos A-O) Table 3: N=4 maser clusters, (Nos 1-4). See also [SVM2001].
in source:	W 75
Ref:	=1986MNRAS.219..145B
by	BAART E.E. , COHEN R.J., DAVIES R.D., NORRIS R.P., ROWLAND P.R.
	Mon. Not. R. Astron. Soc., 219, 145-155 (1986)
	Merlin observations of OH outflow in W75N.
o	Table 1: <[BCD86] Maser A> (Nos A-O). Table 3: <[BCD86] Cluster N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCD98]
[BCD98]	(Benetti+Cappellaro+Danziger+, 1998) (Not yet in Simbad)
Write:	<<[BCD98] NN>>
N:	12
Object:	* (SIMBAD class: Star)
Note:	Table 1, Fig.1: N=12 stars in the field of SN 1994AJ
Ref:	=1998MNRAS.294..448B
by	BENETTI S. , CAPPELLARO E., DANZIGER I.J., TURATTO M., PATAT F., DELLA VALLE M.
	Mon. Not. R. Astron. Soc., 294, 448-456 (1998)
	Supernova 1994aj: a probe for pre-supernova evolution and mass-loss from the progenitor.
o	Table 1: <[BCD98] NN> (Nos 1-12)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BCDSP
BCDSP	(Bica+Claria+Dottori+Santos+Piatti)
Write:	<<BCDSP N>>
N:	8
Object:	Cluster of * + Assoc. (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Table 1: N=8 new Cl* or Assoc. in the LMC among the 624 obj.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1996ApJS..102...57B
by	BICA E. , CLARIA J.J., DOTTORI H., SANTOS J.F.C.Jr, PIATTI A.E.
	Astrophys. J., Suppl. Ser., 102, 57-73 (1996)
	Integrated UBV photometry of 624 star clusters and associations in the Large Magellanic Cloud.
o	Table 1: Some objects are followed by 'w' or 'P1', indicating a direction or a part of the object. Only the whole objects are in SIMBAD
o	Table 1: <BCDSP N> (Nos 1-8)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BCE2005]
[BCE2005]	(Brandl+Clark+Eikenberry+, 2005)= (WIRC)
Write:	<<[BCE2005] NNN>>
N:	57+60+26
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	27 Antennae young star clusters (Table 3) have been detected by HST and the VLA with WIRC. See also [WZ2002] and [NU2000].
in source:	NAME the Antennae
Ref:	=2005ApJ...635..280B
by	BRANDL B.R. , CLARK D.M., EIKENBERRY S.S., WILSON J.C., HENDERSON C.P., BARRY D.J., HOUCK J.R., CARSON J.C., HAYWARD T.L.
	Astrophys. J., 635, 280-289 (2005)
	Deep near-infrared imaging and photometry of the Antennae galaxies with WIRC.
o	Tables 1, 2, 3: <[BCE2005] NNN> N=143 among (Nos 1-234).
=E=	Catalogue in electronic form as J/ApJ/635/280
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BCF
BCF	(Bulge Control Field) (Not yet in Simbad)
*****	Avoid the usage of BCF, prefer [LS2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BCF2017]
[BCF2017]	(Bielby+Crighton+Fumagalli+, 2017)
Write:	<<[BCF2017] JHHMMSS+DDMMSS>> <<[BCF2017] Group>>
N:	13+1
Object:	G + Group of G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT MUSE observations of N=13 galaxies in N=1 galaxy group at z=0.28.
Ref:	=2017MNRAS.468.1373B
by	BIELBY R. , CRIGHTON N.H.M., FUMAGALLI M., MORRIS S.L., STOTT J.P., TEJOS N., CANTALUPO S.
	Mon. Not. R. Astron. Soc., 468, 1373-1386 (2017)
	Probing the intra-group medium of a z = 0.28 galaxy group.
o	Table 1: <[BCF2017] JHHMMSS+DDMMSS> N=13. Paragr. 3: <[BCF2017] Group> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCF85]
[BCF85]	(Buonanno+Corsi+Fusi Pecci+, 1985)= (BCFHZ85) = (Buonanno)
Write:	<<[BCF85] Cluster N NNN>> <<[BCF85] AN NNN>> <<[BCF85] Cluster 3 CNNN>>
N:	58+102+131+129+65+272+127+287
Object:	* in Cl* (SIMBAD class: Star)
Note:	Table 1: * in Cluster 1, (Nos 1-58), format 'Cluster 1 NN' Table 2: * in Cluster 2, (Nos 1-102), format 'Cluster 2 NN' Table 3: * in Cluster 3, (Nos 1-131), format 'Cluster 3 NNN' Table 4: * in Cluster 4, (Nos 1-129), format 'Cluster 4 NNN' Table 5: * in Cluster 5, (Nos 1-65), format 'Cluster 5 NN' Table 6: * in field A1, (Nos 1-272), format 'A1 NNN' Table 7: * in field A2, (Nos 1-127), format 'A2 NNN' Table 8: * in Cluster 3, the prefix 'C' identifies stars with only CCD measurements, (Nos C1-C287), format 'Cluster 3 CNNN' Finding charts.
in source:	NAME Fornax 1
in source:	NAME Fornax 2
in source:	NAME Fornax 3
in source:	NAME Fornax 4
in source:	NAME Fornax 5
Ref:	=1985A&A...152...65B
by	BUONANNO R. , CORSI C.E., FUSI PECCI F., HARDY E., ZINN R.
	Astron. Astrophys., 152, 65-84 (1985)
	Color-magnitude diagrams for the clusters and the field of the Fornax dwarf spheroidal galaxy.
o	Table 1: <[BCF85] Cluster 1 NN> (Nos 1-58). Table 2: <[BCF85] Cluster 2 NNN> (Nos 1-102). Table 3: <[BCF85] Cluster 3 NNN> (Nos 1-131). Table 4: <[BCF85] Cluster 4 NNN> (Nos 1-129). Table 5: <[BCF85] Cluster 5 NN> (Nos 1-65). Table 6: <[BCF85] A1 NNN> (Nos 1-272). Table 7: <[BCF85] A2 NNN> (Nos 1-127). Table 8: <[BCF85] Cluster 3 CNNN> (Nos C1-C287)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCF91]
[BCF91]	(Berger+Cordoni+Fringant+, 1991)
Write:	<<[BCF91] NNNN>>
N:	1221
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Ref:	=1991A&AS...87..389B
by	BERGER J. , CORDONI J.P., FRINGANT A.M., GUIBERT J., MOREAU O., REBOUL H., VANDERRIEST C.
	Astron. Astrophys., Suppl. Ser., 87, 389-418 (1991)
	MAMA astrometry and photometry of 1221 UV-excess objects in 40 square ° at the North Galactic Pole.
o	<[BCF91] NNNN> N=1221
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BCFHZ85
BCFHZ85	(Buonanno+Corsi+Fusi Pecci+Hardy+Zinn, 1985)
*****	Avoid the usage of BCFHZ85, prefer [BCF85]
Origin	of the Acronym: L (1997A&A...317...54J)
Details on Acronym: [BCG2006]
[BCG2006]	(Bradac+Clowe+Gonzalez+, 2006)
Write:	<<[BCG2006] A>> <<[BCG2006] AN>> <<[BCG2006] A DDD.ddddd+DD.dddddd>>
N:	12+29
Object:	G + Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST ACS images: strong-lensing analysis of the 1ES 0657-558 cluster. See also [MSS2001].
Ref:	=2006ApJ...652..937B
by	BRADAC M. , CLOWE D., GONZALEZ A.H., MARSHALL P., FORMAN W., JONES C., MARKEVITCH M., RANDALL S., SCHRABBACK T., ZARITSKY D.
	Astrophys. J., 652, 937-947 (2006)
	Strong and weak lensing united. III. Measuring the mass distribution of the merging galaxy cluster 1ES 0657-558.
o	Fig.1, Table 1: <[BCG2006] A> (Nos A-J), <[BCG2006] AN> = <[BCG2006] A DDD.ddddd+DD.ddddd> N=23.
Ref:	=2009ApJ...706.1201B
by	BRADAC M. , TREU T., APPLEGATE D., GONZALEZ A.H., CLOWE D., FORMAN W., JONES C., MARSHALL P., SCHNEIDER P., ZARITSKY D.
	Astrophys. J., 706, 1201-1212 (2009)
	Focusing cosmic telescopes: exploring redshift z ~ 5-6 galaxies with the bullet cluster 1E0657-56.
o	Table 1: <[BCG2006] A> (Nos K-L) added, <[BCG2006] A DDD.ddddd+DD.ddddd> N=6 added. Table 2: <[BTA2009] DDD.ddddd+DD.ddddd> N=24.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCG2009]
[BCG2009]	(Brusa+Comastri+Gilli+, 2009)= (XMMC)
Write:	<<[BCG2009] JHHMMSS.s+DDMMSS>>
N:	40
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	XMM observations of high-redshift quasars in the COSMOS field.
Ref:	=2009ApJ...693....8B
by	BRUSA M. , COMASTRI A., GILLI R., HASINGER G., IWASAWA K., MAINIERI V., MIGNOLI M., SALVATO M., ZAMORANI G., BONGIORNO A., CAPPELLUTI N., CIVANO F., FIORE F., MERLONI A., SILVERMAN J., TRUMP J., VIGNALI C., CAPAK P., ELVIS M., ILBERT O., IMPEY C., LILLY S.
	Astrophys. J., 693, 8-22 (2009)
	High-redshift quasars in the COSMOS survey: the space density of z > 3 X-ray selected QSOs.
o	Table 1: <[BCG2009] JHHMMSS.s+DDMMSS> N=40.
=E=	Catalogue in electronic form as <J/ApJ/693/8/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCG2010]
[BCG2010]	(Bragaglia+Carretta+Gratton+, 2010)
Write:	<<[BCG2010] bMS>> <<[BCG2010] rMS>>
N:	2
Object:	* (SIMBAD class: Star)
Note:	VLT X-Shooter observations of N=2 main sequence stars (one star on the bluest and the other on the reddest main sequence) in the globular clutser NGC 2808.
in source:	NGC 2808
Ref:	=2010ApJ...720L..41B
by	BRAGAGLIA A. , CARRETTA E., GRATTON R.G., LUCATELLO S., MILONE A., PIOTTO G., D'ORAZI V., CASSISI S., SNEDEN C., BEDIN L.R.
	Astrophys. J., 720L, 41-45 (2010)
	X-shooter observations of main-sequence stars in the globular cluster NGC 2808: first chemical tagging of a he-normal and a he-rich dwarf.
o	Table 1: <[BCG2010] bMS Star> N=1, <[BCG2010] rMS Star> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCG93]
[BCG93]	(Briceno+Calvet+Gomez+, 1993)= (Briceno) = (CIDA)
Write:	<<[BCG93] NN>>
N:	14
Object:	T Tau * (SIMBAD class: TTauri* = T Tauri Star)
Stat:	is completely incorporated in Simbad
Note:	Identif. charts
in source:	NAME Tau-Aur
Ref:	=1993PASP..105..686B
by	BRICENO C. , CALVET N., GOMEZ M., HARTMANN L.W., KENYON S.J., WHITNEY B.A.
	Publ. Astron. Soc. Pac., 105, 686-None (1993)
	First results of the CIDA Schmidt Survey: selected zones in Taurus-Auriga.
o	IRAS 05023+2527 = IRAS 05022+2527
o	<[BCG93] NN> (Nos 1-12).
Ref:	=1999AJ....118.1354B
by	BRICENO C. , CALVET N., KENYON S., HARTMANN L.
	Astron. J., 118, 1354-1368 (1999)
	A large-scale objective-prism and X-ray survey in Taurus-Auriga.
o	Tables 3, 7, 8: <[BCK99] HCl 2 NW-NNa> N=10, <[BCK99] HCl 2 SE-Na> N=7, <[BCK99] L1537-NN> N=5 among 14, <[BCK99] L1538-N> N=2 among 5, <[BCK99] L1544A-N> N=2 among 9, <[BCK99] L1544B-NNa> N=4 among 10. Table 4: <[BCG93] NN> (Nos 13-14) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCH2000]
[BCH2000]	(Battinelli+Capuzzo-Dolcetta+Hodge+, 2000) (Not yet in Simbad)
Write:	<<[BCH2000] NGC 7217 NNN>> <<[BCH2000] NGC 1058 NN>> <<[BCH2000] UGC 12732 NNN>>
N:	149+35+108
Object:	Young Star Grouping (SIMBAD class: Unknown = Object of Unknown Nature)
in source:	NGC 7217
in source:	NGC 1058
in source:	UGC 12732
Ref:	=2000A&A...357..437B
by	BATTINELLI P. , CAPUZZO-DOLCETTA R., HODGE P.W., VICARI A., WYDER T.K.
	Astron. Astrophys., 357, 437-442 (2000)
	Large scale star formation in galaxies. I. The spirals NGC 7217, NGC 1058 and UGC 12732. Young star groupings in spirals.
o	Table 1: <[BCH2000] NGC 7217 NNN> (Nos 1-149). Table 2: <[BCH2000] NGC 1058 NN> (Nos 1-35). Table 3: <[BCH2000] UGC 12732 NNN> (Nos 1-108).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCH2001]
[BCH2001]	(Ball+Crawford+Hunstead+, 2001) (Not yet in Simbad)
Write:	<<[BCH2001] N>>
N:	3
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=3 background objects in the field of SN 1987A, used for calibrating the flux density of the SN.
Ref:	=2001ApJ...549..599B
by	BALL L. , CRAWFORD D.F., HUNSTEAD R.W., KLAMER I., McINTYRE V.J.
	Astrophys. J., 549, 599-607 (2001)
	Radio supernova 1987A at 843 MHz.
o	Fig.1: <[BCH2001] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCH2002]
[BCH2002]	(Borys+Chapman+Halpern+, 2002)= (HDFSMM)
Write:	<<[BCH2002] MMSS+MMSS>>
N:	12
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SCUBA map of the HDF. In the format 'MMSS.s-MMSS', relative to 12h and +62deg, (2000 coordinates). See also [BCH2003], [BSC2004].
in source:	NAME HDFN
Ref:	=2002MNRAS.330L..63B
by	BORYS C. , CHAPMAN S.C., HALPERN M., SCOTT D.
	Mon. Not. R. Astron. Soc., 330, 63-67 (2002)
	A SCUBA scan-map of the Hubble Deep Field : measuring the bright end of the submillimetre source counts.
o	Table 1: <[BCH2002] MMSS+MMSS> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCH2003]
[BCH2003]	(Borys+Chapman+Halpern+, 2003)= (SMM)
Write:	<<[BCH2003] SMM JHHMMSS+DDMMSS>>
N:	39
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SCUBA super-map of the HDFN. See also [BCH2002], [BSC2004].
in source:	NAME HDFN
Ref:	=2003MNRAS.344..385B
by	BORYS C. , CHAPMAN S., HALPERN M., SCOTT D.
	Mon. Not. R. Astron. Soc., 344, 385-398 (2003)
	The Hubble Deep Field North SCUBA Super-map - I. Submillimetre maps, sources and number counts.
o	In reference list: Barger, Cowie, Richards (Ba00) is 2000, AJ, vol. 119 , p. 2092 instead of 2002
o	Table 2: <[BCH2003] SMM JHHMMSS+DDMMSS> N=39.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCH2005]
[BCH2005]	(Benn+Carballo+Holt+, 2005)
Write:	<<[BCH2005] QSO J1624+3758 abs N.NNNN>>
N:	16
Object:	Absorber
Note:	WHT ISIS spectroscopic observations of the absorption-line QSO J1624+3758.
Ref:	=2005MNRAS.360.1455B
by	BENN C.R. , CARBALLO R., HOLT J., VIGOTTI M., GONZALEZ-SERRANO J.I., MACK K.-H., PERLEY R.A.
	Mon. Not. R. Astron. Soc., 360, 1455-1470 (2005)
	Unusual high-redshift radio broad absorption-line quasar 1624+3758.
o	Quasar 1624+3758 = QSO J1624+3758
o	Table 4: <[BCH2005] QSO J1624+3758 abs N.NNNN> N=16.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCH2007]
[BCH2007]	(Brogan+Chandler+Hunter+, 2007)
Write:	<<[BCH2007] SMA N>> <<[BCH2007] HW2-SMA>> <<[BCH2007] HW3c-SMA>>
N:	4+2
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	Submillimeter Array (SMA) observations of Cep A East region.
in source:	Cep A:Cep A East = Cep A East
Ref:	=2007ApJ...660L.133B
by	BROGAN C.L. , CHANDLER C.J., HUNTER T.R., SHIRLEY Y.L., SARMA A.P.
	Astrophys. J., 660L, 133-136 (2007)
	Arcsecond-scale kinematic and chemical complexity in Cepheus A East.
o	Fig.1, Table 2: <[BCH2007] SMA N> (Nos 1-4), <[BCH2007] HW2-SMA> N=1, <[BCH2007] HW3c-SMA> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCH2008]
[BCH2008]	(Brunner+Cappelluti+Hasinger+, 2008)
Write:	<<[BCH2008] NNNN>>
N:	409
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton observations of the Lockman Hole. See also [MBC2005], [MBH2002].
in source:	NAME Lockman Hole
Ref:	=2008A&A...479..283B
by	BRUNNER H. , CAPPELLUTI N., HASINGER G., BARCONS X., FABIAN A.C., MAINIERI V., SZOKOLY G.
	Astron. Astrophys., 479, 283-300 (2008)
	XMM-Newton observations of the Lockman Hole: X-ray source catalogue and number counts.
o	Table 3: <[BCH2008] NNNN> N=409 among (Nos 5-2838).
=E=	Catalogue in electronic form as <J/A+A/479/283/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCH2009]
[BCH2009]	(Baumgardt+Cote+Hilker+, 2009)
Write:	<<[BCH2009] SNN>>
N:	19
Object:	Poss. RGB* (SIMBAD class: RGB*_Candidate = Red Giant Branch star Candidate)
Note:	Keck I HIRES observations of candidate RGB stars in NGC 2419.
in source:	NGC 2419
Ref:	=2009MNRAS.396.2051B
by	BAUMGARDT H. , COTE P., HILKER M., REJKUBA M., MIESKE S., DJORGOVSKI S.G., STETSON P.
	Mon. Not. R. Astron. Soc., 396, 2051-2060 (2009)
	The velocity dispersion and mass-to-light ratio of the remote halo globular cluster NGC2419.
o	Correct coordinates for [BCH2009] S10, are, as in Figure 2 : 07:38:05.98+38:52:05.5; J2000 and not the ones given in Table 1.
o	Table 1: <[BCH2009] SNN> N=19 among (Nos S2-S41).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCH2012]
[BCH2012]	(Bartlett+Coe+Haberl+, 2012)
Write:	<<[BCH2012] NNN>>
N:	81
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton EPIC observations N=81 X-ray sources in the field of the Phoenix dwarf galaxy.
in source:	NAME Phe Dwarf Galaxy
Ref:	=2012MNRAS.422.2302B
by	BARTLETT E.S. , COE M.J., HABERL F., McBRIDE V.A., CORBET R.H.D.
	Mon. Not. R. Astron. Soc., 422, 2302-2313 (2012)
	The search for high-mass X-ray binaries in the Phoenix dwarf galaxy.
o	Fig. 2, Tables 3+A1: <[BCH2012] NNN> N=5+76 among (Nos 1-101).
=E=	Catalogue in electronic form as J/MNRAS/422/2302
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCH97]
[BCH97]	(Bomans+Chu+Hopp, 1997)
Write:	<<[BCH97] SN>> <<[BCH97] SGS N>> <<[BCH97] SB N>> <<[BCH97] Fil NN>>
N:	7+5+9+38
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC, Einstein IPC and HRI, HST WFPC2 observations Text, and Table 1: N=7 sources (Nos S1-S7) Table A1: N=5 SuperGiant Shells, format 'SGS N' and N=9 SuperBubbles, format 'SB N' Table A2: N=38 Filaments, format 'Fil NN' Maps in Figs 3 and 5
in source:	NGC 4449
Ref:	=1997AJ....113.1678B
by	BOMANS D.J. , CHU Y.-H., HOPP U.
	Astron. J., 113, 1678-1690 (1997)
	Hot interstellar gas in the irregular galaxy NGC 4449.
o	Table 1: <[BCH97] SN> (Nos S1-S7). Table A1: <[BCH97] SGS N> (Nos 1-5), <[BCH97] SB N> (Nos 1-9). Table A2: <[BCH97] Fil NN> (Nos 1-38)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCI89]
[BCI89]	(Barbon+Ciatti+Iijima+, 1989)
Write:	<<[BCI89] SN 1983R NN>> <<[BCI89] SN 1983U N>>
N:	14+6
Object:	* (SIMBAD class: Star)
Note:	Asiago systematic study of supernovae. Reference stars in the field of 2 SN.
Ref:	=1989A&A...214..131B
by	BARBON R. , CIATTI F., IIJIMA T., ROSINO L.
	Astron. Astrophys., 214, 131-138 (1989)
	Photographic and spectroscopic observations of three type Ia supernovae : 1982W, 1983R, and 1983U.
o	Table 2, Fig.2: <[BCI89] SN 1983R NN> (Nos 1-14). Table 5, Fig.5: <[BCI89] SN 1983U N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCJ2008]
[BCJ2008]	(Bennert+Canalizo+Jungwiert+, 2008) (Not yet in Simbad)
Write:	<<[BCJ2008] PHL 909 a>> <<[BCJ2008] PKS 0736+01 a>> <<[BCJ2008] PG 0923+2011 a>> <<[BCJ2008] PG 0923+2011 N>> <<[BCJ2008] OX 169 a>>
N:	10+3+6+2+3
Object:	G + Arc (SIMBAD class: Galaxy)
Note:	HST ACS images of the fields of N=5 galaxies.
Ref:	=2008ApJ...677..846B
by	BENNERT N. , CANALIZO G., JUNGWIERT B., STOCKTON A., SCHWEIZER F., PENG C.Y., LACY M.
	Astrophys. J., 677, 846-857 (2008)
	Evidence for merger remnants in early-type host galaxies of low-redshift QSOs.
o	PKS 0736+201 is a misprint (0726+01 or 0923+201)
o	Fig.4, Appendix: <[BCJ2008] PHL 909 a> (Nos a-j), <[BCJ2008] PKS 0736+01 a> (Nos a-c), <[BCJ2008] PG 0923+201 a> (Nos a-f), <[BCJ2008] PG 0923+201 N> (Nos 1-2), <[BCJ2008] OX 169 a> (Nos a-c).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCJ2017]
[BCJ2017]	(Banerji+Carilli+Jones+, 2017)
Write:	<<[BCJ2017] G1234-W>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ALMA Cycle 3 band 3 CO(3-2) line observations of N=2 millimetre-bright galaxies detected in the field of view of the quasar ULAS J1234+0907 at z=2.503.
in source:	ULAS J123427.52+090754.1
Ref:	=2017MNRAS.465.4390B
by	BANERJI M. , CARILLI C.L., JONES G., WAGG J., McMAHON R.G., HEWETT P.C., ALAGHBAND-ZADEH S., FERUGLIO C.
	Mon. Not. R. Astron. Soc., 465, 4390-4405 (2017)
	The discovery of gas-rich, dusty starbursts in luminous reddened quasars at z ~ 2.5 with ALMA.
o	Table 4: <[BCJ2017] G1234-W> (Nos S and N).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCK2003]
[BCK2003]	(Berger+Cowie+Kulkarni+, 2003)
Write:	<<[BCK2003] GN>> <<[BCK2003] VLA JHHMMSS.ss+DDMMSS.s>> <<[BCK2003] SMM JHHMMm+DDMM>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	SCUBA and VLA observations. Study of GRB 000418 host galaxy. N=2 galaxies (Nos G1-G2) with 2 VLA sources respectively at the position of each galaxy, and a SMM source at the position of G1. G1 is the host galaxy.
Ref:	=2003ApJ...588...99B
by	BERGER E. , COWIE L.L., KULKARNI S.R., FRAIL D.A., AUSSEL H., BARGER A.J.
	Astrophys. J., 588, 99-112 (2003)
	A submillimeter and radio survey of γ-ray burst host galaxies: a glimpse into the future of star formation studies.
o	Fig.2: <[BCK2003] GN> (Nos G1-G2) = <[BCK2003] VLA JHHMMSS.ss+DDMMSS.s> N=2. Text: <[BCK2003] SMM JHHMMm+DDMM> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCK2005]
[BCK2005]	(Begum+Chengalur+Karachentsev+, 2005)
Write:	<<[BCK2005] HIZSS003A>>
N:	2
Object:	G in Pair (SIMBAD class: GinPair = Galaxy in Pair of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	GMRT HI observations of the dwarf galaxy HIZSS3: the main galaxy, here HIZSS003A, has a smaller companion HIZSS003B.
Ref:	=2005MNRAS.359L..53B
by	BEGUM A. , CHENGALUR J.N., KARACHENTSEV I.D., SHARINA M.E.
	Mon. Not. R. Astron. Soc., 359, 53-57 (2005)
	Resolving the mystery of the dwarf galaxy HIZSS003.
o	<[BCK2005] HIZSS003A> (Nos A, B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCK2006]
[BCK2006]	(Brisken+Carrillo-Barragan+kIRTZ+, 2006)
Write:	<<[BCK2006] N>>
N:	8
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 20cm observations of the field of PSR B1800-21.
Ref:	=2006ApJ...652..554B
by	BRISKEN W.F. , CARRILLO-BARRAGAN M., KURTZ S., FINLEY J.P.
	Astrophys. J., 652, 554-558 (2006)
	Proper motion of pulsar B1800-21.
o	Table 2: <[BCK2006] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCK2009]
[BCK2009]	(Bendo+Clements+Khan, 2009)= ([BCK2009a]) (Not yet in Simbad)
Write:	<<[BCK2009] WN>> <<[BCK2009] WN>>
N:	2+5
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Note:	VLT VIMOS integral-field spectroscopy of the Southern and Northern nuclei (SN and NN) of the ultraluminous infrared galaxy pair IRAS 19254-7245 (the Superantennae).
in source:	NAME Superantennae
Ref:	=2009MNRAS.399L..29B
by	BENDO G.J. , CLEMENTS D.L., KHAN S.A.
	Mon. Not. R. Astron. Soc., 399L, 29-33 (2009)
	Spectroscopically and spatially resolved optical line emission in the Superantennae (IRAS 19254-7245).
o	Table 1, Fig. 3: <[BCK2009] WN> (Nos SN, NN), <[BCK2009] WN> (Nos S1-S4, N1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCK2009a]
[BCK2009a]	(Bendo+Clements+Khan, 2009) (Not yet in Simbad)
*****	Avoid the usage of [BCK2009a], prefer [BCK2009]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCK2009b]
[BCK2009b]	(Boquien+Calzetti+Kennicutt+, 2009)
Write:	<<[BCK2009b] NGC NNNN-A-NN>>
N:	324
Object:	Star Forming Region (SIMBAD class: PartofG = Part of a Galaxy)
Note:	KPNO 2.1m and CTIO 1.5m observations of eight nearby galaxies. Use of GALEX and SINGS archives.
in source:	NGC 628 = M 74
in source:	NGC 2403
in source:	NGC 3031 = M 81
in source:	NGC 5055 = M 63
in source:	NGC 5194 = M 51
in source:	NGC 5236 = M 83
in source:	NGC 5457 = M 101
in source:	NGC 7793
Ref:	=2009ApJ...706..553B
by	BOQUIEN M. , CALZETTI D., KENNICUTT R., DALE D., ENGELBRACHT C., GORDON K.D., HONG S., LEE J.C., PORTOUW J.
	Astrophys. J., 706, 553-570 (2009)
	Star-forming or starbursting? The ultraviolet conundrum.
o	Table 4: <[BCK2009b] NGC NNNN-A-NN> N=324.
=E=	Catalogue in electronic form as <J/ApJ/706/553/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCK2022]
[BCK2022]	(Barnes+Chandar+Kreckel+, 2022)
Write:	<<[BCK2022] NN>>
N:	40
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	N=40 HII regions in the nearby star-forming galaxy NGC 1672. Use of data from the PHANGS-HST and PHANGS-MUSE surveys.
in source:	NGC 1672
Ref:	=2022A&A...662L...6B
by	BARNES A.T. , CHANDAR R., KRECKEL K., GLOVER S.C.O., SCHEUERMANN F., BELFIORE F., BIGIEL F., BLANC G.A., BOQUIEN M., DEN BROK J., CONGIU E., CHEVANCE M., DALE D.A., DEGER S., KRUIJSSEN J.M.D., EGOROV O.V., EIBENSTEINER C., EMSELLEM E., GRASHA K., GROVES B., KLESSEN R.S., HANNON S., HASSANI H., LEE J.C., LEROY A.K., LOPEZ L.A., McLEOD A.F., PAN H., SANCHEZ-BLAZQUEZ P., SCHINNERER E., SORMANI M.C., THILKER D.A., UBEDA L., WATKINS E.J., WILLIAMS T.G.
	Astron. Astrophys., 662L, 6-6 (2022)
	Linking stellar populations to H II regions across nearby galaxies. I. Constraining pre-supernova feedback from young clusters in NGC 1672.
o	Table A.1: <[BCK2022] NN> (Nos 0-39).
=E=	Catalogue in electronic form as J/A+A/662/L6
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [BCK99]
[BCK99]	(Briceno+Calvet+Kenyon+, 1999)
Write:	<<[BCK99] HCl 2 WW-NNa>> <<[BCK99] L1537-NN>> <<[BCK99] L1538-N>> <<[BCK99] L1544A-N>> <<[BCK99] L1544B-NNa>>
N:	28
Object:	(X) (SIMBAD class: X = X-ray Source)
in source:	NAME Tau-Aur
Ref:	=1999AJ....118.1354B
by	BRICENO C. , CALVET N., KENYON S., HARTMANN L.
	Astron. J., 118, 1354-1368 (1999)
	A large-scale objective-prism and X-ray survey in Taurus-Auriga.
o	Tables 3, 7, 8: <[BCK99] HCl 2 NW-NNa> N=10, <[BCK99] HCl 2 SE-Na> N=7, <[BCK99] L1537-NN> N=5 among 14, <[BCK99] L1538-N> N=2 among 5, <[BCK99] L1544A-N> N=2 among 9, <[BCK99] L1544B-NNa> N=4 among 10. Table 4: <[BCG93] NN> (Nos 13-14) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BCL
BCL	(Boulesteix+Courtes+Laval+)
*****	Avoid the usage of BCL, prefer BCLMP
Origin	of the Acronym: L (2001A&A...373..438H)
Details on Acronym: [BCL2000]
[BCL2000]	(Bonnet-Bidaud+Colas+Lecacheux, 2000)
Write:	<<[BCL2000] NN>>
N:	32
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Stars in the field of Sirius. See also [BG91].
Ref:	=2000A&A...360..991B
by	BONNET-BIDAUD J.M. , COLAS F., LECACHEUX J.
	Astron. Astrophys., 360, 991-996 (2000)
	Search for companions around Sirius.
o	Table 2: [BG91] N (Nos 1-9).
o	Table 1: <[BCL2000] NN> (Nos 1-32).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCL2001]
[BCL2001]	(Boyle+Croom+Lewis+, 2001)
Write:	<<[BCL2001] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of SN 2001O.
Ref:	=2001IAUC.7574....1B
by	BOYLE B.J. , CROOM S.M., LEWIS I.J., POGSON J., GLAZEBROOK K.
	IAU Circ., 7574, 1-None (2001)
	Supernova 2001O in anonymous galaxy.
o	<[BCL2001] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCL2009]
[BCL2009]	(Bravo-Alfaro+Caretta+Lobo+, 2009)
Write:	<<[BCL2009] NN>>
N:	42
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Sample of brightes blue galaxies in A85. Use of archival SuperCOSMOS data.
in source:	ACO 85
Ref:	=2009A&A...495..379B
by	BRAVO-ALFARO H. , CARETTA C.A., LOBO C., DURRET F., SCOTT T.
	Astron. Astrophys., 495, 379-387 (2009)
	Galaxy evolution in Abell 85. I. Cluster substructure and environmental effects on the blue galaxy population.
o	Table 1: <[BCL2009] NN> (Nos 1-42).
=E=	Catalogue in electronic form as J/A+A/495/379
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCL74]
[BCL74]	(Boulesteix+Courtes+Laval+, 1974)
*****	Avoid the usage of [BCL74], prefer BCLMP
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCL98]
[BCL98]	(Burud+Courbin+Lidman+, 1998)
Write:	<<[BCL98] RX J0911.4+0551 AN>> <<[BCL98] RX J0911.4+0551 A>>
N:	4+1
Object:	QSO component + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=4 images of the QSO RX J0911.4+0551, (Nos A1-A3, B), and N=1 Lensing galaxy 'No. G' See also ref. 1998ApJ...501L...5B. See also [BSL97]
in source:	RX J0911.0+0551
Ref:	=1998Msngr..92...29B
by	BURUD I. , COURBIN F., LIDMAN C., MEYLAN G., MAGAIN P., JAUNSEN A.O., HJORTH J., OSTENSEN R., ANDERSEN M.I., CLASEN J.W., STABELL R., REFSDAL S.
	The Messenger, 92, 29-32 (1998)
	RX J0911.4+0551: a complex quadruply imaged gravitationally lensed QSO.
o	Table 1: <[BCL98] RX J0911.4+0551 AN> (Nos A1-A3, B), <[BCL98] RX J0911.4+0551 G> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BCLMP
BCLMP	(Boulesteix+Courtes+Laval+Monnet+Petit)= (B) = (BCL) = ([BCL74])
Write:	<<BCLMP NNNNA>> <<BCLMP NNNNW>>
N:	369+30
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Table 1: (Nos 1-101) are identical to [CC65], BCLMP supersedes [CC65]. See also CPDSP.
in source:	M 33 = NGC 598
Ref:	=1974A&A....37...33B
by	BOULESTEIX J. , COURTES G., LAVAL G., MONNET G., PETIT H.
	Astron. Astrophys., 37, 33-48 (1974)
	An optical study of M 33: I. Morphology of the gas.
o	Table 1: (Nos 1-101) are identical to [CC65] 1 to 101.
o	Table 1: <BCLMP NNNNA>, N=369, (Nos 1-6, 7A-7B, 8A-8B, 9-49, 49A, 50-88, 89A-89B, 90-94, 95A-95B, 96-101, 200-289, 290A-290C, 301-302, 601-645, 646A-646B, 647-760, 1001-1008, 1501-1502).
Ref:	=2002ApJ...568..679W
by	WILLNER S.P. , NELSON-PATEL K.
	Astrophys. J., 568, 679-688 (2002)
	Neon abundances in the H II regions of M33.
o	Table 1: <BCLMP NNNA> (Nos 680B, 680C) added, <BCLMP NNNW> (Nos 87E, 88W, 740W, 638E, 638N) added.
Ref:	=2007A&A...470..843M
by	MAGRINI L. , CORBELLI E., GALLI D.
	Astron. Astrophys., 470, 843-855 (2007)
	The building up of the disk galaxy M33 and the evolution of the metallicity gradient.
o	Table 1: <BCLMP NNNA> (No. 915B) added.
Ref:	=2007A&A...470..865M
by	MAGRINI L. , VILCHEZ J.M., MAMPASO A., CORRADI R.L.M., LEISY P.
	Astron. Astrophys., 470, 865-874 (2007)
	The metallicity gradient of M 33: chemical abundances of HII regions.
o	Table 1 BCLMP 84 is a misprint for BCLMP 284.
o	Table 1: <BCLMP NNNA> N=16 added. Table 1: <LGC-HII NN> (Nos 1-13).
Origin	of the Acronym: L (1978A&A....62...51V)
Details on Acronym: [BCM2000]
[BCM2000]	(Bertoldi+Carilli+Menten+, 2000)
Write:	<<[BCM2000] JHHMMSS+DDMM>>
N:	2
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=2 new mm sources towards ACO 2125.
Ref:	=2000A&A...360...92B
by	BERTOLDI F. , CARILLI C.L., MENTEN K.M., OWEN F., DEY A., GUETH F., GRAHAM J.R., KREYSA E., LEDLOW M., LIU M.C., MOTTE F., REICHERTZ L., SCHILKE P., ZYLKA R.
	Astron. Astrophys., 360, 92-98 (2000)
	Three high-redshift millimeter sources and their radio and near-infrared identifications.
o	T.1: first source is [ELG99] CFRS 14A = CUDSS 14.1.
o	Table 1: <[BCM2000] JHHMMSS+DDMM> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCM2001]
[BCM2001]	(Barger+Cowie+Mushotzky+, 2001)
Write:	<<[BCM2001] NN>>
N:	20
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra hard X-ray image of the HDS field SSA 13. Finding charts in Fig.2.
Ref:	=2001AJ....121..662B
by	BARGER A.J. , COWIE L.L., MUSHOTZKY R.F., RICHARDS E.A.
	Astron. J., 121, 662-682 (2001)
	The nature of the hard X-ray background sources: optical, near-infrared, submillimeter, and radio properties.
o	Table 1: <[BCM2001] NN> (Nos 0-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCM2009]
[BCM2009]	(Baxter+Covey+Muench+, 2009)= ([BCM2009a])
Write:	<<[BCM2009] DDD.ddddddd+DD.ddddddd>>
N:	97
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	MMT Hectochelle spectroscopy of N=97 stars in the open cluster NGC 2264.
in source:	NGC 2264
Ref:	=2009AJ....138..963B
by	BAXTER E.J. , COVEY K.R., MUENCH A.A., FURESZ G., REBULL L., SZENTGYORGYI A.H.
	Astron. J., 138, 963-974 (2009)
	The distance to NGC 2264.
o	Table 2: <[BCM2009] DDD.ddddddd+DD.ddddddd> N=97.
=E=	Catalogue in electronic form as <J/AJ/138/963/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCM2009a]
[BCM2009a]	(Baxter+Covey+Muench+, 2009) (Not yet in Simbad)
Note:	Distance sample to determine the distance to NGC 2264.
*****	Avoid the usage of [BCM2009a], prefer [BCM2009]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCM2009b]
[BCM2009b]	(Baume+Carraro+Momany, 2009)
Write:	<<[BCM2009b] NNNNN>>
N:	34310
Object:	* (SIMBAD class: Star)
Note:	CTIO SMARTS 1.0-telescope observations of a rich and complex field in the Galactic Plane towards l~305deg and b~0deg.
Ref:	=2009MNRAS.398..221B
by	BAUME G. , CARRARO G., MOMANY Y.
	Mon. Not. R. Astron. Soc., 398, 221-232 (2009)
	A study of the galactic plane towards l = 305°.
o	Table 2: <[BCM2009b] NNNNN> (Nos 1-34310).
=E=	Catalogue in electronic form as <J/MNRAS/398/221/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCM2013]
[BCM2013]	(Bernieri+Campana+Massaro+, 2013)
Write:	<<[BCM2013] J1418+3542>>
N:	[BCM2013]
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	N=1 gamma-ray source in the Fermi-LAT sky. Use of archival Fermi-LAT sky images.
Ref:	=2013A&A...551L...5B
by	BERNIERI E. , CAMPANA R., MASSARO E., PAGGI A., TRAMACERE A.
	Astron. Astrophys., 551L, 5-5 (2013)
	A new flaring high-energy γ-ray source.
o	<[BCM2013] J1418+3542> N=1.
o	SDSS J14186+3542 is SDSS J141840.08+354102.0 in Simbad.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
History	of this Acronym: replaced by Fermi
Details on Acronym: [BCM2016]
[BCM2016]	(Beltran+Cesaroni+Moscadelli+, 2016)
Write:	<<[BCM2016] NNa>> <<[BCM2016] Feature NN>>
N:	17+14
Object:	(Rad) + maser (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLA continuum observations at 2cm, 1.3cm, 6cm, 3.6cm and 7mm of the high-mass star-forming region G35.20-0.74N. See also [GHL2003].
in source:	NAME G 35.2-0.74N
Ref:	=2016A&A...593A..49B
by	BELTRAN M.T. , CESARONI R., MOSCADELLI L., SANCHEZ-MONGE A., HIROTA T., KUMAR M.S.N.
	Astron. Astrophys., 593A, 49-49 (2016)
	Binary system and jet precession and expansion in G35.20-0.74N.
o	Tables 2-3, Fig. 1,5: <[BCM2016] NNa> (Nos 1-16, 8a-8b). Table 4: <[BCM2016 Feature NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCM2019]
[BCM2019]	(Braga+Contreras Ramos+Minniti+, 2019)= ([BCM2019a])
Write:	<<[BCM2019] b333 NNN NNNNNN>>
N:	1019
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	N=1019 periodic variable stars in the central most tile (b333) of the VISTA Variables in the Via Lactea (VVV) Survey.
in source:	NAME Galactic Center
Ref:	=2019A&A...625A.151B
by	BRAGA V.F. , CONTRERAS RAMOS R., MINNITI D., FERREIRA LOPES C.E., CATELAN M., MINNITI J.H., NIKZAT F., ZOCCALI M.
	Astron. Astrophys., 625A, 151-151 (2019)
	New type II Cepheids from VVV data towards the Galactic center.
o	Tables 2-3: <[BCM2019] b333 NNN NNNNNN> N=1019.
=E=	Catalogue in electronic form as <J/A+A/625/A151/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCM2019a]
[BCM2019a]	(Braga+Contreras Ramos+Minniti+, 2019)
*****	Avoid the usage of [BCM2019a], prefer [BCM2019]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCM2019b]
[BCM2019b]	(Bhatawdekar+Conselice+Margalef-Bentabol+, 2019)
Write:	<<[BCM2019b] NNNN>>
N:	10+8
Object:	G (SIMBAD class: Galaxy)
Note:	N=10 galaxies at z∼8 and N=8 galaxies at z∼9 in the field of the strong-lensing cluster MCS J0416.0-2403 and the associated parallel field. Use of HST data from the Hubble Frontier Fields (HFF) program. Use of archival VLT HAWK-I and Spitzer IRAC data.
in source:	MCS J0416.1-2403
Ref:	=2019MNRAS.486.3805B
by	BHATAWDEKAR R. , CONSELICE C.J., MARGALEF-BENTABOL B., DUNCAN K.
	Mon. Not. R. Astron. Soc., 486, 3805-3830 (2019)
	Evolution of the galaxy stellar mass functions and UV luminosity functions at z = 6-9 in the Hubble Frontier Fields.
o	Tables A1-A2: <[BCM2019b] NNNN> N=10+8 among (Nos 126-2674).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCM85]
[BCM85]	(Bohannan+Conti+Massey, 1985)= (BEM)
Write:	<<[BCM85] NN>>
N:	82
Object:	Em. Obj. (SIMBAD class: EmObj = Emission Object)
in source:	M 33 = NGC 598
Ref:	=1985AJ.....90..600B
by	BOHANNAN B. , CONTI P.S., MASSEY P.
	Astron. J., 90, 600-605 (1985)
	A grism search of Messier 33 for emission-line objects.
o	<[BCM85] NN> N=82
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCM89]
[BCM89]	(Bajaja+Cappa de Nicolau+Martin+, 1989)= ([BCM89a])
Write:	<<[BCM89] LLL+BB+VVV>> <<[BCM89] LLL.l+BB+VVV>> <<[BCM89] LLL+BB.b+VVV>> <<[BCM89] LLL.l+BB.b+VVV>>
N:	18
Object:	HVC (SIMBAD class: HVCld = High-velocity Cloud)
Stat:	is completely incorporated in Simbad
Note:	Tables I, II, III: N=18 selected objects with higher sensitivity. HI maps See also HVC
Ref:	=1989A&AS...78..345B
by	BAJAJA E. , CAPPA DE NICOLAU C.E., MARTIN M.C., MORRAS R., OLANO C.A., POPPEL W.G.L.
	Astron. Astrophys., Suppl. Ser., 78, 345-362 (1989)
	A survey of several southern high-velocity complexes.
o	Tables I, II, III: <[BCM89] LLL+BB+VVV>, <[BCM89] LLL.l+BB.b+VVV> N=18.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCM89a]
[BCM89a]	(Bajaja+Cappa de Nicolau+Martin+, 1989)
*****	Avoid the usage of [BCM89a], prefer [BCM89]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCM89b]
[BCM89b]	(Bassani+Coe+Malkan+, 1989)
Write:	<<[BCM89b] N>>
N:	6
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=6 objects (2 galaxies, 1 radio, 3 stars) in the error box of IRAS 16524+3930. Finding chart in Fig.1.
Ref:	=1989ApJ...344..726B
by	BASSANI L. , COE M.J., MALKAN M.A., MANDOLESI N., PARTRIDGE B., SPINOGLIO L.
	Astrophys. J., 344, 726-733 (1989)
	A new narrow-line Seyfert 1 galaxy: IRAS 1652+395.
o	Fig.1, Table 2: <[BCM89b] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCM90]
[BCM90]	(Bachiller+Cernicharo+Martin-Pintado+, 2000)
Write:	<<[BCM90] U-star>> <<[BCM90] B>> <<[BCM90] BN>> <<[BCM90] R>> <<[BCM90] RN>> <<[BCM90] BW>> <<[BCM90] RW>>
N:	1+2+8+2
Object:	Feature (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	p.178: N=1 'U-star', the letter 'U' stands for 'Unseen', Hypothetical exciting star of the outflow. In the outflow, the gaz is concentrated in 2 lobes, blueshifted lobe 'B' and redshifted lobe 'R'. Redshifted emission is divided into 2 features 'RN' and 'RS'. Bullets (Nos B1-B4) have their counterparts (Nos R1-R4) at symmetric positions with respect to the U-star.
in source:	LDN 1448
Ref:	=1990A&A...231..174B
by	BACHILLER R. , CERNICHARO J., MARTIN-PINTADO J., TAFALLA M., LAZAREFF B.
	Astron. Astrophys., 231, 174-186 (1990)
	High-velocity molecular bullets in a fast bipolar outflow near L 1448/IRS 3.
o	L 1448/IRS 3 = [BC86b] LDN 1448 IRS 3.
o	Text, p.178: <[BCM90] U-star> N=1. Figs 8, 9: <[BCM90] A> (Nos R, B), <[BCM90] AW> (Nos RN, RS), <[BCM90] AN> (Nos R1-R4, B1-B4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCP2004]
[BCP2004]	(Bolton+Cotter+Pooley+, 2004)
Write:	<<[BCP2004] 9C JHHMM+DDMM>>
N:	51
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio (VLA and OVRO) and optical (Palomar) observations of N=51 sources which are not in the 9C catalog.
Ref:	=2004MNRAS.354..485B
by	BOLTON R.C. , COTTER G., POOLEY G.G., RILEY J.M., WALDRAM E.M., CHANDLER C.J., MASON B.S., PEARSON T.J., READHEAD A.C.S.
	Mon. Not. R. Astron. Soc., 354, 485-521 (2004)
	The radio source population at high frequency: follow-up of the 15-GHz 9C survey.
o	Table 2: <[BCP2004] 9C JHHMM+DDMM> N=51.
=E=	Catalogue in electronic form as J/MNRAS/354/485
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCP2007]
[BCP2007]	(Block+COmbes+Puerari+, 2007) (Not yet in Simbad)
Write:	<<[BCP2007] N>>
N:	7
Object:	* (SIMBAD class: Star)
Note:	Keck spectroscopy and SST analysis pf M 33. N=7 target posible Carbon stars.
in source:	M 33 = NGC 598
Ref:	=2007A&A...471..467B
by	BLOCK D.L. , COMBES F., PUERARI I., FREEMAN K.C., STOCKTON A., CANALIZO G., JARRETT T.H., GROESS R., WORTHEY G., GEHRZ R.D., WOODWARD C.E., POLOMSKI E.F., FAZIO G.G.
	Astron. Astrophys., 471, 467-474 (2007)
	Keck spectroscopy and Spitzer space telescope analysis of the outer disk of the Triangulum spiral galaxy M 33.
o	Fig.2, Table 1: <[BCP2007] N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCP93]
[BCP93]	(Bresolin+Capaccioli+Piotto, 1993)
Write:	<<[BCP93] FN HN>> <<[BCP93] DN HN>>
N:	39
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	In the format, the letter F or D stand for fields, the letter H for HII region.
in source:	NGC 3109
Ref:	=1993AJ....105.1779B
by	BRESOLIN F. , CAPACCIOLI M., PIOTTO G.
	Astron. J., 105, 1779-1792 (1993)
	The dwarf galaxy NGC 3109. I. The data.
o	Table 4: <[BCP93] FN HN> N=28, <[BCP93] DN HN> N=11.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCP98]
[BCP98]	(Bhargavi+Cowsik+Pati+, 1998) (Not yet in Simbad)
Write:	<<[BCP98] ANN>> <<[BCP98] BNN>>
N:	25+30
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Objects in the field of GRB 910814: (Nos A1-A25) are brighter objects, (Nos B1-B30) are fainter. Image in Fig.1
Ref:	=1998BASI...26..597B
by	BHARGAVI S.G. , COWSIK R., PATI A.K., SAGAR R.
	Bull. Astron. Soc. India, 26, 597-601 (1998)
	CCD imaging of γ ray burster fields.
o	Fig.1: <[BCP98] ANN> (Nos A1-A25, B1-B30).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCP99]
[BCP99]	(Benetti+Cappellaro+Pastorello+, 1999)
Write:	<<[BCP99] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=1, host galaxy of SN 1999EY
Ref:	=1999IAUC.7310R...1B
by	BENETTI S. , CAPPELLARO E., PASTORELLO A., PREVEDELLO M., SALVO M., TURATTO M., DANZIGER J., MAZZALI P., RIZZI L., PATAT F.
	IAU Circ., 7310, 1-None (1999)
	Supernova 1999ey in anonymous galaxy.
o	<[BCP99] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BCR
BCR	(Barger+Cowie+Richards)
*****	Avoid the usage of BCR, prefer [BCR2000]
Origin	of the Acronym: L (2003MNRAS.342..759A)
Details on Acronym: [BCR2000]
[BCR2000]	(Barger+Cowie+Richards, 2000)= (BCR)
Write:	<<[BCR2000] NN>>
N:	70
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=69 high-redshift dusty galaxies from the [R2000] catalogue in the flanking fields of HDFN. See also [WCB2004].
Ref:	=2000AJ....119.2092B
by	BARGER A.J. , COWIE L.L., RICHARDS E.A.
	Astron. J., 119, 2092-2109 (2000)
	Mapping the evolution of high-redshift dusty galaxies with submillimeter observations of a radio-selected sample.
o	Table 1: misprint in Decl for Nos 2, 14, 18, 27. Par. 2.3, blazar 0954+685 misprint for 658.
o	Table 1: <[BCR2000] NN> (Nos 0-69).
Origin	of the Acronym: L (2003MNRAS.342..759A)
Details on Acronym: [BCR2006]
[BCR2006]	(Berger+Cenko+Rau, 2006)
Write:	<<[BCR2006] SN>> <<[BCR2006] GN>> <<[BCR2006] G*>>
N:	4+2+1
Object:	* G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Keck and Gemini observations of the field GRB 060502B. G* is the putative host galaxy of the GRB.
Ref:	=2006GCN..5071....1B
by	BERGER E. , CENKO S.B., RAU A.
	GRB Coordinates Network, Circular Service, 5071, 1-None (2006)
	GRB 060502b: Gemini imaging and spectroscopy.
o	<[BCR2006] SN> (No. S1), <[BCR2006] GN> (No. G1).
Ref:	=2006GCN..5077....1P
by	PRICE P.A. , BERGER E., FOX D.B., CENKO S.B., RAU A.
	GRB Coordinates Network, Circular Service, 5077, 1-None (2006)
	GRB 060502b: Second epoch Gemini observations.
o	<[BCR2006] SN> (No. S2) added.
Ref:	=2007ApJ...654..878B
by	BLOOM J.S. , PERLEY D.A., CHEN H.-W., BUTLER N., PROCHASKA J.X., KOCEVSKI D., BLAKE C.H., SZENTGYORGYI A., FALCO E.E., STARR D.L.
	Astrophys. J., 654, 878-884 (2007)
	A putative early-type host galaxy for GRB 060502B: implications for the progenitors of short-duration hard-spectrum bursts.
o	Fig.1, Table 2: <[BCR2006] SN> (Nos S3-S4) added, <[BCR2006] GN> (No. G2) added, <[BCR2006] G*> added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCR2013]
[BCR2013]	(Boone+Clement+Richard+, 2013)
Write:	<<[BCR2013] LN>>
N:	4
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Stat:	is completely incorporated in Simbad
Note:	APEX LABOCA 870µm observations of N=4 lensed images in the field of the galaxy cluster ACO S 1063.
in source:	ACO S 1063 = RXC J2248.0-4431
Ref:	=2013A&A...559L...1B
by	BOONE F. , CLEMENT B., RICHARD J., SCHAERER D., LUTZ D., WEISS A., ZEMCOV M., EGAMI E., RAWLE T.D., WALTH G.L., KNEIB J.-P., COMBES F., SMAIL I., SWINBANK A.M., ALTIERI B., BLAIN A.W., CHAPMAN S., DESSAUGES-ZAVADSKY M., IVISON R.J., KNUDSEN K.K., OMONT A., PELLO R., PEREZ-GONZALEZ P.G., VALTCHANOV I., VAN DER WERF P., ZAMOJSKI M.
	Astron. Astrophys., 559L, 1-1 (2013)
	An extended Herschel drop-out source in the center of AS 1063: a normal dusty galaxy at z = 6.1 or SZ substructures ?
o	Fig. 2: <[BCR2013] LN> (Nos L1-L4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCR2014]
[BCR2014]	(Borissova+Chene+Ramirez Alegria+, 2014)
Write:	<<[BCR2014] CLNNN N>> <<[BCR2014] CLNNNobjN>> (not recognised by Simbad, but found in literature)
N:	90 (SIMBAD class: Star)
Note:	Use of data from the ESO Public Survey "VISTA Variables in the Via Lactea" (VVV) to discover and analyse obscured star clusters in the direction of the inner Galactic disk and bulge.
Ref:	=2014A&A...569A..24B
by	BORISSOVA J. , CHENE A.-N., RAMIREZ ALEGRIA S., SHARMA S., CLARKE J.R.A., KURTEV R., NEGUERUELA I., MARCO A., AMIGO P., MINNITI D., BICA E., BONATTO C., CATELAN M., FIERRO C., GEISLER D., GROMADZKI M., HEMPEL M., HANSON M.M., IVANOV V.D., LUCAS P., MAJAESS D., MONI BIDIN C., POPESCU B., SAITO R.K.
	Astron. Astrophys., 569A, 24-24 (2014)
	New galactic star clusters discovered in the VVV survey. Candidates projected on the inner disk and bulge.
o	Table 1: <VVV CLNNN> N=58 among (Nos 106 to 163). Table 3: <[BCR2014] CLNNN NN> N=90.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCR73]
[BCR73]	(Barbon+Ciatti+Rosino, 1973)
Write:	<<[BCR73] NGC NNNN a>>
N:	36+41
Object:	* (SIMBAD class: Star)
Note:	Asiago systematic study of supernovae. Reference stars in the field of 5 and 4 galaxies host of SN
Ref:	=1973MmSAI..44...65B
by	BARBON R. , CIATTI F., ROSINO L.
	Mem. Soc. Astron. Ital., 44, 65-85 (1973)
	Observations of five supernovae 1970-71.
o	Table I, Fig.1: <[BCR73] NGC 7619 a> (Nos a-i, l). Table III, Fig.3: <[BCR73] NGC 2968 a> (Nos a-i). Table V, Fig.5: <[BCR73] NGC 4165 a> (Nos a-h). Table VII, Fig.7: <[BCR73] NGC 5055 a> (Nos a-i, l). Table IX, Fig.10: <[BCR73] NGC 6384 a> (Nos a-i).
Ref:	=1973A&A....29...57B
by	BARBON R. , CIATTI F., ROSINO L.
	Astron. Astrophys., 29, 57-67 (1973)
	Light curves and characteristics of recent supernovae.
o	Table 2, Fig.1: <[BCR73] NGC 5457 a> (Nos a-p). Table 4, Fig.4: <[BCR73] NGC 3147 a> (Nos a-g). Table 6, Fig.6: <[BCR73] NGC 2841 a> (Nos a-i). Table 9, Fig.8: <[BCR73] NGC 4254 a> (Nos a-h).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCR82]
[BCR82]	(Barbon+Ciatti+Rosino, 1982)
Write:	<<[BCR82] NGC 6946 A>> <<[BCR82] NGC 4536 a>>
N:	11+9
Object:	* (SIMBAD class: Star)
Note:	Asiago systematic study of supernovae. Reference stars in the field of 2 galaxies host of SN. Stars 'A' in the field of NGC 6946 are from a private communication of De Vaucouleurs (1981).
Ref:	=1982A&A...116...35B
by	BARBON R. , CIATTI F., ROSINO L.
	Astron. Astrophys., 116, 35-42 (1982)
	Two bright supernovae in NGC 6946 and NGC 4536.
o	Table 1, Fig.1: <[BCR82] NGC 6946 A> N=11 among (Nos B-T). Table 4, Fig.6: <[BCR82] NGC 4536 a> (Nos a-i).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BCS
BCS	(Blanco Cosmology Survey) >>>>>> New acronym being registered
Object:	?
Auth.:	TUCKER D.L.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [BCS2001]
[BCS2001]	(Bianchi+Catanzaro+Scuderi+, 2001)= ([BCS2001a])
Write:	<<[BCS2001] M33-NNNN>>
N:	7
Object:	* (SIMBAD class: Star)
Note:	CFHT spectroscopic observations. N=7 massive stars in M 33, from an HST WFPC2 photometric sample. The authors used a different format for other stars in Paper II: [CBS2003].
in source:	M 33 = NGC 598
Ref:	=2001PASP..113..697B
by	BIANCHI L. , CATANZARO G., SCUDERI S., HUTCHINGS J.B.
	Publ. Astron. Soc. Pac., 113, 697-702 (2001)
	Spectroscopy of massive stars in NGC 6822 and M33.
o	Table 2: <[BCS2001] M33-NNNN> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCS2001a]
[BCS2001a]	(Bianchi+Catanzaro+Scuderi+, 2001)
*****	Avoid the usage of [BCS2001a], prefer [BCS2001]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCS2001b]
[BCS2001b]	(Buckley+Coe+Stevens+, 2001) (Not yet in Simbad)
Write:	<<[BCS2001b] A>>
N:	7
Object:	* (SIMBAD class: Star)
Note:	ROSAT PSPC archives: Finding chart of 1WGA J0053.8-7226: N=7 stars in the field.
Ref:	=2001MNRAS.320..281B
by	BUCKLEY D.A.H. , COE M.J., STEVENS J.B., VAN DER HEYDEN K., ANGELINI L., WHITE N., GIOMMI P.
	Mon. Not. R. Astron. Soc., 320, 281-288 (2001)
	Multiwaveband studies of the hard ROSAT SMC transient 1WGA J0053.8-7226: a new X-ray pulsar.
o	p. 282 RX J0054.9-7210 misprint for RX J0054.9-7226 ?
o	Fig.3: <[BCS2001b] A> (Nos A-G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCS2002]
[BCS2002]	(Balogh+Couch+Smail+, 2002)
Write:	<<[BCS2002] NNNN>>
N:	525
Object:	H-alpha G (SIMBAD class: Galaxy)
Note:	LDSS+ spectrograph on the AAT and HST observations. H-alpha survey of ACO 1689. See also [FED2000].
in source:	ACO 1689
Ref:	=2002MNRAS.335...10B
by	BALOGH M.L. , COUCH W.J., SMAIL I., BOWER R.G., GLAZEBROOK K.
	Mon. Not. R. Astron. Soc., 335, 10-22 (2002)
	An Hα survey of the rich cluster A 1689.
o	Table 1: <[BCS2002] NNNN> N=525 among (Nos 3-5171).
=E=	Catalogue in electronic form as J/MNRAS/335/10
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCS2004]
[BCS2004]	(Briley+Cohen+Stetson, 2004)
Write:	<<[BCS2004] M 13 MMSSs+MMSS>> <<[BCS2004] M 71 CMMSSs+MMSS>>
N:	51+103+76
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Keck LRIS observations of M 13 and M 71. In Tables 3, 4, coordinates in the format are 2000 coordinates with RA 16h and Dec +36deg. In Table 5 coordinates in the format are 1950 coordinates with RA 19h and Dec +18deg. See also [CBS2002].
in source:	M 13 = NGC 6205
in source:	M 71 = NGC 6838
Ref:	=2004AJ....127.1579B
by	BRILEY M.M. , COHEN J.G., STETSON P.B.
	Astron. J., 127, 1579-1587 (2004)
	The chemical inhomogeneity of faint M13 stars: carbon and nitrogen abundances.
o	Table 4: The stars are not M5 subgiants (misprint) but M13 subgiants. In T.3, 4: coordinates in the format are 2000 coordinates with RA 16h and Dec +36°. In T.5: coordinates in the format are 1950 coordinates with RA 19h and Dec +18°.
o	Tables 3, 4: <[BCS2004] M 13 MMSSs+MMSS> N=51+103. Table 5: <[BCS2004] M 71 CMMSSs+MMSS> N=76.
=E=	Catalogue in electronic form as J/AJ/127/1579
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCS2006]
[BCS2006]	(Bernardi+Carretti+Sault+, 2006)
Write:	<<[BCS2006] F-NN>>
N:	18+15
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA 1.4GHz polarimetric observations of 2 fields of the DASI (Degree Angular Scale Interferometer) experiment.
Ref:	=2006MNRAS.370.2064B
by	BERNARDI G. , CARRETTI E., SAULT R.J., CORTIGLIONI S., POPPI S.
	Mon. Not. R. Astron. Soc., 370, 2064-2070 (2006)
	1.4-GHz polarimetric observations of the two fields imaged by the DASI experiment.
o	Table 2: <[BCS2006] 1-NN> (Nos 1-1 to 1-18). Table 3: <[BCS2006] 2-NN> (Nos 2-1 to 2-15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCS2009]
[BCS2009]	(Beasley+Cenarro+Strader+, 2009) (Not yet in Simbad)
Write:	<<[BCS2009] VCC1261 GCNNN>> <<[BCS2009] VCC1528 GCNN>>
N:	13+12
Object:	GlCl + Star (SIMBAD class: GlobCluster = Globular Cluster)
Note:	Keck I LRIS spectroscopy of globular clusters in VCC 1261 and VCC 1528. See also [BSB2006] for globular clusters in VCC 1087..
in source:	VCC 1261
in source:	VCC 1528
Ref:	=2009AJ....137.5146B
by	BEASLEY M.A. , CENARRO A.J., STRADER J., BRODIE J.P.
	Astron. J., 137, 5146-5153 (2009)
	Evidence for the disky origin of luminous Virgo dwarf ellipticals from the kinematics of their globular cluster systems.
o	Table 1: <[BCS2009] VCC1261 GCNNN> N=13 among (Nos 101-308), <[BCS2009] VCC1528 GCNN> N=12 among (Nos 1-17).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCS2011]
[BCS2011]	(Banerji+Chapman+Smail+, 2011)
Write:	<<[BCS2011] sxdfNNNN>> <<[BCS2011] lockNNN>> <<[BCS2011] c03.NN>> <<[BCS2011] c03.1420>>
N:	12+5+1 +3
Object:	G (SIMBAD class: Galaxy)
Note:	Keck II DEIMOS observations of luminous starburst galaxies in the SXDF, Lockman Hole and CFRS 03 fields.
in source:	NAME SXDF
in source:	NAME Lockman Hole
Ref:	=2011MNRAS.418.1071B
by	BANERJI M. , CHAPMAN S.C., SMAIL I., ALAGHBAND-ZADEH S., SWINBANK A.M., DUNLOP J.S., IVISON R.J., BLAIN A.W.
	Mon. Not. R. Astron. Soc., 418, 1071-1088 (2011)
	Luminous starbursts in the redshift desert at z~ 1–2: star formation rates, masses and evidence for outflows.
o	Table 2: <[BCS2011] sxdfNNNN> N=12 among (Nos 490-1300), <[BCS2011] lockNNN> N=5 among (Nos 218-517), <[BCS2011] c03.1420> N=1, <[BCS2011] c03.NN> (Nos 14, 56, 62).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCS2012]
[BCS2012]	(Basa+Cuby+Savaglio+, 2012)= ([BCS2012a])
Write:	<<[BCS2012] GRB 080913 host>>
N:	1 (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT X-Shooter observations of the field of GRB 080913.
Ref:	=2012A&A...542A.103B
by	BASA S. , CUBY J.G., SAVAGLIO S., BOISSIER S., CLEMENT B., FLORES H., LE BORGNE D., MAZURE A.
	Astron. Astrophys., 542A, 103-103 (2012)
	Constraining the nature of the most distant γ-ray burst host galaxies.
o	<[BCS2012] GRB 080913 host> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCS2012a]
[BCS2012a]	(Basa+Cuby+Savaglio+, 2012)
*****	Avoid the usage of [BCS2012a], prefer [BCS2012]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCS2012b]
[BCS2012b]	(Briere+Cantin+Spekkens, 2012)
Write:	<<[BCS2012b] NN>>
N:	51
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Mont Megantic 1.6m telescope observations of N=51 giant HII regions in the spiral arms and bar of NGC 5430.
in source:	NGC 5430
Ref:	=2012MNRAS.425..261B
by	BRIERE E. , CANTIN S., SPEKKENS K.
	Mon. Not. R. Astron. Soc., 425, 261-272 (2012)
	Properties of the giant HII regions and bar in the nearby spiral galaxy NGC5430.
o	Table 2: <[BCS2012b] NN> (Nos 1-51).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCS2015]
[BCS2015]	(Bragaglia+Carretta+Sollima+, 2015)
Write:	<<[BCS2015] tNNNNN>>
N:	48+64
Object:	* (SIMBAD class: Star)
Note:	VLT FLAMES UVES+GIRAFFE spectroscopy of N=48+64 stars in the Globular Cluster NGC 6139.
in source:	NGC 6139
Ref:	=2015A&A...583A..69B
by	BRAGAGLIA A. , CARRETTA E., SOLLIMA A., DONATI P., D'ORAZI V., GRATTON R.G., LUCATELLO S., SNEDEN C.
	Astron. Astrophys., 583A, 69-69 (2015)
	NGC 6139: a normal massive globular cluster, or a first-generation dominated cluster? Clues from the light elements.
o	Table A.1: <[BCS2015] tNNNNN> N=48 among (Nos t00261-t06169). Table A.2: <[BCS2015] tNNNNN> N=64 among (Nos t00187-t04132).
=E=	Catalogue in electronic form as J/A+A/583/A69
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCS89]
[BCS89]	(Bothun+Cladwell+Schombert, 1989)= (B)
Write:	<<[BCS89] NNN>>
N:	124
Object:	dw. Ell. G (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table V
in source:	Centaurus Cluster = ACO 3526
Ref:	=1989AJ.....98.1542B
by	BOTHUN G.D. , CALDWELL N., SCHOMBERT J.M.
	Astron. J., 98, 1542-1553 (1989)
	The use of dwarf elliptical galaxies as distance indicators: the relative distances between Virgo, Fornax, and Centaurus.
o	(Erratum) + erratum Astron. J. 99, 736
o	Table V: <[BCS89] NNN> N=124
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCS92]
[BCS92]	(Bergeron+Cristiani+Shaver, 1992)
Write:	<<[BCS92] 0102-190 NN>> <<[BCS92] 0102-190 GN>> <<[BCS92] 2206-199 NN>> <<[BCS92] 2206-199 GN>>
N:	17+3+18+4
Object:	QSO + G (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	Table 2: QSO in the two fields '0102-190' and '2206-199', format '0102-190 NN' (Nos 1-18), and format '2206-199 NN' (Nos 1-19) cross-id. with the galaxies 'GN' in each fields. Table 3: galaxies in each field, format '0102-190 GN' (Nos G1-G3) format '2206-199 GN' (Nos G1-G4) See also [B86b], [BB86b], [BDK87], [B88], [BBK88], [BB91], [GB97]
Ref:	=1992A&A...257..417B
by	BERGERON J. , CRISTIANI S., SHAVER P.A.
	Astron. Astrophys., 257, 417-424 (1992)
	Discovery of z about 1 galaxies causing quasar absorption lines.
o	Table 2: <[BCS92] 0102-190 NN> (Nos 1-18), <[BCS92] 2206-199 NN> (Nos 1-19). Tables 3, 4: <[BCS92] 0102-190 GN> (Nos G1-G3), <[BCS92] 2206-199 GN> (Nos G1-G4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCS95]
[BCS95]	(Blum+Carr+Sellgren+, 1995)
Write:	<<[BCS95] N-NN>>
N:	39+39+40
Object:	M Giant (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 2: format '1-NN' N=39, format '2-NN' N=39, format '3-NN' N=40.
in source:	NAME Gal Center
Ref:	=1995ApJ...449..623B
by	BLUM R.D. , CARR J.S., SELLGREN K., TERNDRUP D.M.
	Astrophys. J., 449, 623-634 (1995)
	M giant kinematics in off-axis fields between 150 and 300 parsecs from the Galactic Center.
o	standard star 301 (p. 627) not in SIMBAD
o	Table 2: <[BCS95] 1-NN> (Nos 1-39), <[BCS95] 2-NN> (Nos 1-39), <[BCS95] 3-NN> (Nos 1-40)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCS98]
[BCS98]	(Barger+Cowie+Sanders+, 1998)= (SMM)
Write:	<<[BCS98] SMM JHHMMm-DDMM>> <<[BCS98] SMM JHHMMSS.s+DDMMSS.s>>
N:	3
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	N=1 submm source in ACO 370: 'SMM J02399-0136' 1st found in 1997ApJ...490L...5S: [BCS98] SMM J02399-0136 = [SIB97] J023953.0-013506 See also [SIB97] N=1 submm source in Lockman hole: 'SMM J103402.3+574625.0' N=1 submm source in SSA 13: 'SMM J131232.1+424428.0' See also [BCS99].
in source:	ACO 370
in source:	NAME Lockman Hole
in source:	SSA 13
Ref:	=1998Natur.394..248B
by	BARGER A.J. , COWIE L.L., SANDERS D.B., FULTON E., TANIGUCHI Y., SATO Y., KAWARA K., OKUDA H.
	Nature, 394, 248-251 (1998)
	Submillimetre-wavelength detection of dusty star-forming galaxies at high redshift.
o	coordinates of SMM in ACO 370 are J2000 coordinates, °. of declinaison are -01
o	<[BCS98] SMM J02399-0136>, <[BCS98] SMM J103402.3+574625.0>, <[BCS98] SMM J131232.1+424428.0>, N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCS99]
[BCS99]	(Barger+Cowie+Sanders, 1999)= ([BCS99a])
Write:	<<[BCS99] JHHMMSS.s+DDMMSS>>
N:	21
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SCUBA data on 3 Hawaii Deep Survey fields: SSA 13, SSA 17, SSA 22, and Lockman hole. See also [BCS98], [ELG99].
Ref:	=1999ApJ...518L...5B
by	BARGER A.J. , COWIE L.L., SANDERS D.B.
	Astrophys. J., 518, 5-8 (1999)
	Resolving the submillimeter background: the 850 micron galaxy counts.
o	Table 1: <[BCS99] JHHMMSS.s+DDMMSS> N=21.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCS99a]
[BCS99a]	(Barger+Cowie+Sanders, 1999)
*****	Avoid the usage of [BCS99a], prefer [BCS99]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCS99b]
[BCS99b]	(Barger+Cowie+Smail+, 1999)
Write:	<<[BCS99b] Cl HHMM+DD ANNa>> <<[BCS99b] ACO NNNN ANa>>
N:	50
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Keck images are used to study possible optical counterparts of SMM sources in 7 clusters. In ACO 370, objects L1 and L2 are also designated as [ISL98] L1 and L2. In ACO 1835: The SMM source consist of 2 optical components J1 and J2. [BCS99b] ACO 1835 J1 has many subcomponents: 5 images J1a to J1e, and J1n, an object north of ACO 1835 J1 also designated as [ISF2001] ACO 1835 J1n. See also [FRA2004].
in source:	ClG 0024+1652 = HMS 0024+1654
in source:	ClG 2244-02
in source:	ClG 0939+4713 = ACO 851
in source:	ClG 0440+02 = 1E 0440.5+0204
in source:	ACO 370
in source:	ACO 1835
in source:	ACO 2390
Ref:	=1999AJ....117.2656B
by	BARGER A.J. , COWIE L.L., SMAIL I., IVISON R.J., BLAIN A.W., KNEIB J.-P.
	Astron. J., 117, 2656-2665 (1999)
	Redshift distribution of the faint submillimeter galaxy population.
o	Table 2, col(3): <[BCS99b] ACO 370 LN> (Nos L1-L5), <[BCS99b] Cl 0024+16 MNN> N=8 among (Nos M1-M11), <[BCS99b] Cl 0939+47 HN> (Nos H1, H4), <[BCS99b] ACO 1835 JN> (Nos J1-J4), <[BCS99b] Cl 2244-02 PN> (Nos P1-P4), <[BCS99b] Cl 0440+02 AN> (Nos N1, N5), <[BCS99b] ACO 2390 KN> (Nos K2, K3).
Ref:	=1999MNRAS.308.1061S
by	SMAIL I. , IVISON R.J., KNEIB J.-P., COWIE L.L., BLAIN A.W., BARGER A.J., OWEN F.N., MORRISON G.
	Mon. Not. R. Astron. Soc., 308, 1061-1068 (1999)
	The discovery of ERO counterparts to faint submillimetre galaxies.
o	Table 2: <[BCS99b] Cl 0939+47 HN> (No. H5), <[BCS99b] Cl 0440+02 AN> (No. N4).
Ref:	=2000MNRAS.315..209I
by	IVISON R.J. , SMAIL I., BARGER A.J., KNEIB J.-P., BLAIN A.W., OWEN F.N., KERR T.H., COWIE L.L.
	Mon. Not. R. Astron. Soc., 315, 209-222 (2000)
	The diversity of SCUBA-selected galaxies.
o	Table 2: <[SIB98] SMM J14010+0253> added. Table 2: <[BCS99b] ACO 1835 JN> (Nos J5-J8).
Ref:	=2001ApJ...561L..45I
by	IVISON R.J. , SMAIL I., FRAYER D.T., KNEIB J.-P., BLAIN A.W.
	Astrophys. J., 561, 45-49 (2001)
	Locating the starburst in the SCUBA galaxy SMM J14011+0252.
o	Fig.1: <[ISF2001] ACO 1835 J1n> = <[BCS99b] ACO 1835 J1n> N=1.
Ref:	=2002MNRAS.335L..17C
by	CHAPMAN S.C. , SMAIL I., IVISON R.J., BLAIN A.W.
	Mon. Not. R. Astron. Soc., 335, 17-21 (2002)
	The effect of lensing on the identification of SCUBA galaxies.
o	Table 1, last col.: N2 850.1 = [SFD2002] N2 1, ERO: M12 = [BCS99b] Cl 0024+16 M12, ERO: N4 = [BCS99b] Cl 0440+02 N4, HDF 850.1 = [HSD98] F850.1. SSA22 850.2 is one of the [CLS2001] object, but which one?
o	Table 1: <[CSI2002b] SMM JHHMMm+DDMM> N=5. Table 1: <[BCS99b] Cl 0024+16 MNN> (No. M12) added.
Ref:	=2002ApJ...577L..79L
by	LEDLOW M.J. , SMAIL I., OWEN F.N., KEEL W.C., IVISON R.J., MORRISON G.E.
	Astrophys. J., 577, 79-82 (2002)
	Gemini multi-object spectrograph observations of SCUBA galaxies behind A851.
o	<[BCS99b] Cl 0939+47 HN> (Nos H6-H8) added. <[LSO2002] SMM JHHMMm+DDMM> N=2.
Ref:	=2004AJ....127..728F
by	FRAYER D.T. , REDDY N.A., ARMUS L., BLAIN A.W., SCOVILLE N.Z., SMAIL I.
	Astron. J., 127, 728-735 (2004)
	Near-infrared colors of submillimeter-selected galaxies.
o	Table 2: <[FRA2004] AN> (Nos A1-A3, B1). Table 2: <[BCS99b] ACO 1835 J1a> (No. J1a) added, <[BCS99b] Cl 2244-02 ANa> (Nos P1a, P1b, P7) added, <[BCS99b] ACO 2390 ANa> (Nos K3a, K3b) added.
Ref:	=2005AJ....129...53M
by	MOTOHARA K. , TAKATA T., IWAMURO F., ETO S., SHIMA T., MOCHIDA D., MAIHARA T., NAKANISHI K., KASHIKAWA N.
	Astron. J., 129, 53-60 (2005)
	Nature of the strongly lensed submillimeter galaxy SMM J14011+0252.
o	Fig.4, Table 5: <[BCS99b] ACO 1835 J1a> (Nos J1b to J1e) added. Fig.5, Table 5: <[MTI2005] HA Cloud> N=1, <[MTI2005] HA-a> (Nos HA-a to HA-d).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BCT
BCT	(Bregman+Cox+Tomisaka)
*****	Avoid the usage of BCT, prefer [BCT93]
Origin	of the Acronym: L (2000MNRAS.319...17L)
Details on Acronym: [BCT93]
[BCT93]	(Bregman+Cox+Tomisaka, 1993)= (BCT)
Write:	<<[BCT93] NN>>
N:	10
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations.
in source:	IC 342
Ref:	=1993ApJ...415L..79B
by	BREGMAN J.N. , COX C.V., TOMISAKA K.
	Astrophys. J., 415, 79-82 (1993)
	X-ray emission from the starburst galaxy IC 342.
o	Table 1: <[BCT93] NN> (Nos 1-10)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCV94]
[BCV94]	(Barth +Cepa+Vilchez+, 1994)
Write:	<<[BCV94] 3-NN>> <<[BCV94] 5-N>>
N:	28+8
Object:	HII + Assoc. (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 3: format '3-NN', N=28 HII regions in NGC 4861 Table 5: format '5-N', N=8 emissionless associations in NGC 4861
in source:	NGC 4861
Ref:	=1994AJ....108.2069B
by	BARTH C.S. , CEPA J., VILCHEZ J.M., DOTTORI H.A.
	Astron. J., 108, 2069-2077 (1994)
	CCD imaging of NGC 4861: ionized gas properties and stellar formation.
o	Table 3: <[BCV94] 3-NN> N=28, Table 5: <[BCV94] 5-N> N=8
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCW2007]
[BCW2007]	(Barger+Cowie+Wang, 2007)
Write:	<<[BCW2007] JHHMMSS.ss+DDMMSS.ss>>
N:	12
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 1.4GHz observations of the HDF-N. N=12 bilobal sources without obvious counterparts.
Ref:	=2007ApJ...654..764B
by	BARGER A.J. , COWIE L.L., WANG W.-H.
	Astrophys. J., 654, 764-781 (2007)
	The microjansky radio galaxy population.
o	Table 1: <[BCW2007] JHHMMSS.ss+DDMMSS.ss> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCW2008]
[BCW2008]	(Barger+Cowie+Wang, 2008)
Write:	<<[BCW2008] NNNN>> <<[BCW2008] DDD.dddddd+DD.ddddd>>
N:	6909+1199+1046+2907
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST ACS GOODS North observations.
Ref:	=2008ApJ...689..687B
by	BARGER A.J. , COWIE L.L., WANG W.-H.
	Astrophys. J., 689, 687-708 (2008)
	A highly complete spectroscopic survey of the GOODS-N field.
o	Table 1: <[BCW2008] NNNN> (Nos 1-6909). Tables 2-4: <[BCW2008] DDD.dddddd+DD.ddddd> N=1199+1046+2907.
=E=	Catalogue in electronic form as J/ApJ/689/687
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BCZ2021]
[BCZ2021]	(Boettcher+Chen+Zahedy+, 2021)
Write:	<<[BCZ2021] CUBS0111z057 GNNN>> <<[BCZ2021] CUBS0111z057_GNNN>> (not recognised by Simbad, but found in literature)
N:	9
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Magellan LDSS-3C and IMACS observations of N=9 galaxies around a damped-Lymanα absorber at z=0.576 in the line of sight of QSO J0111-0316, as part of the Cosmic Ultraviolet Baryon Survey (CUBS).
Ref:	=2021ApJ...913...18B
by	BOETTCHER E. , CHEN H.-W., ZAHEDY F.S., COOPER T.J., JOHNSON S.D., RUDIE G.C., CHEN M.C., PETITJEAN P., CANTALUPO S., COOKSEY K.L., FAUCHER-GIGUERE C.-A., GREENE J.E., LOPEZ S., MULCHAEY J.S., PENTON S.V., PUTMAN M.E., RAFELSKI M., RAUCH M., SCHAYE J., SIMCOE R.A., WALTH G.L.
	Astrophys. J., 913, 18-18 (2021)
	The Cosmic Ultraviolet Baryon Survey (CUBS). II. Discovery of an H_{2}-bearing DLA in the vicinity of an early-type galaxy at z = 0.576.
o	Figs 5-6, Table 4: <[BCZ2021] CUBS0111z057 GNNN> N=9 among (Nos G41-G576).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: BD
BD	(Bonner Durchmusterung)= DM = SD
Write:	<<BD +DD NNNNNA>> <<BD +DD NNNNNa>>
N:	324188
Object:	* (SIMBAD class: Star)
Note:	Southern part: delta > -22deg, (Nos -2 1 to -22 6265). Northern part: delta > -1deg, (Nos -1 1 to +89 38). Reprinted in reduced size, Dummler Verlag, Bonn, 1949, 1951A. Reedition: NASA Ref. Publ. 1297 Vol. I, II, 1993. Catalogues I/83/ and I/84/, superseded by I/122/.
Ref:	=1886BD....C......0S
by	SCHOENFELD E.
	Eds Marcus and Weber's Verlag, Bonn, 0-None (1886)
	Bonner Durchmusterung des sudlichen Himmels.
o	<BD+DD NNNNNA> N=134833.
Ref:	=1903BD....C......0A
by	ARGELANDER F.
	Eds Marcus and Weber's Verlag, Bonn, 0-None (1903)
	Bonner Durchmusterung des nordlichen Himmels.
o	revised by KUSTNER F.
o	<BD+DD NNNNNA>
=E=	Catalogue in electronic form as I/119
=E=	Catalogue in electronic form as I/122
Details on Acronym: BD
BD	(Battinelli+Demers)
Note:	Young Assoc. betw. MC
*****	Avoid the usage of BD, prefer ICA
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BD2000]
[BD2000]	(Battinelli+Demers, 2000)
Write:	<<[BD2000] Pegasus CNN>> <<[BD2000] DDO 210 CNN>>
N:	40+3
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Note:	See also [ADK2000], [DB2002], [LDB2002], [BDL2003], [DBL2003], [DBL2003b], [BD2004a], [BD2004b], [DBL2004].
in source:	NAME Pegasus Galaxy
in source:	NAME Aquarius Dwarf Galaxy = DDO 210
Ref:	=2000AJ....120.1801B
by	BATTINELLI P. , DEMERS S.
	Astron. J., 120, 1801-1807 (2000)
	A carbon star survey of the Local Group dwarf galaxies. II. Pegasus, DDO 210, and Tucana.
o	Table 4: <[BD2000] Pegasus CNN> (Nos C01-C40). Table 5: <[BD2000] DDO 210 CNN> (Nos C01-C03).
=E=	Catalogue in electronic form as J/AJ/120/1801
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BD2004a]
[BD2004a]	(Battinelli+Demers, 2004)
Write:	<<[BD2004a] NNN>>
N:	149
Object:	C* (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Note:	CFH12K wide field camera observations. See also [ADK2000], [BD2000], [DB2002], [LDB2002], [BDL2003], [DBL2003], [DBL2003b], [BD2004b], [BD2004c], [DBL2004].
in source:	DDO 221 = WLM Galaxy
Ref:	=2004A&A...416..111B
by	BATTINELLI P. , DEMERS S.
	Astron. Astrophys., 416, 111-118 (2004)
	Carbon star survey of Local Group galaxies. X. Wolf-Lundmark-Melotte a galaxy with an extreme C/M ratio.
o	Table 2: <[BD2004a] NNN> (Nos 1-149).
=E=	Catalogue in electronic form as J/A+A/416/111
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BD2004b]
[BD2004b]	(Battinelli+Demers, 2004)
Write:	<<[BD2004b] NNN>>
N:	145
Object:	C* (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Note:	CFH12K observations. See also [ADK2000], [BD2000], [DB2002], [LDB2002], [BDL2003], [DBL2003], [DBL2003b], [BD2004a], [BD2004c], [DBL2004].
in source:	NGC 185
Ref:	=2004A&A...417..479B
by	BATTINELLI P. , DEMERS S.
	Astron. Astrophys., 417, 479-486 (2004)
	Carbon star survey of Local Group galaxies. IX. The spheroidal galaxy NGC 185.
o	Table 2: <[BD2004b] NNN> (Nos 1-145).
=E=	Catalogue in electronic form as J/A+A/417/479
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BD2004c]
[BD2004c]	(Battinelli+Demers, 2004)
Write:	<<[BD2004c] NNN>>
N:	288
Object:	C* (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Note:	CFH12K observations. See also [ADK2000], [BD2000], [DB2002], [LDB2002], [BDL2003], [DBL2003], [DBL2003b], [BD2004a], [BD2004b], [DBL2004].
in source:	NGC 147
Ref:	=2004A&A...418...33B
by	BATTINELLI P. , DEMERS S.
	Astron. Astrophys., 418, 33-40 (2004)
	Carbon star survey in the Local Group. VIII. Probing the stellar halo of NGC 147.
o	Table 2: <[BD2004c] NNN> (Nos 1-288).
=E=	Catalogue in electronic form as J/A+A/418/33
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BD2004d]
[BD2004d]	(Bonamente+Dixon, 2004)
Write:	<<[BD2004d] QSO J2136-6224 abs N.NNNN>>
N:	1
Object:	Absorber
Note:	FUSE observations of the Syfert G 2MASX J21362313-6224008 = QSO J2136-6224. Absorption lines are forming a system at z=0.0578 in the line of sight of the galaxy.
Ref:	=2004ApJ...609..597B
by	BONAMENTE M. , DIXON W.V.D.
	Astrophys. J., 609, 597-602 (2004)
	FUSE observations of galactic and intrinsic absorption in the spectrum of the Seyfert 1 galaxy 2MASX J21362313-6224008.
o	Text: <[BD2004d] QSO J2136-6224 abs 0.0578> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BD2005]
[BD2005]	(Battinelli+Demers, 2005)
Write:	<<[BD2005] NN>>
N:	15
Object:	C* (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Note:	TNG observations of N=15 carbon stars in the outer disk of M 31.
in source:	M 31 = NGC 224
Ref:	=2005A&A...430..905B
by	BATTINELLI P. , DEMERS S.
	Astron. Astrophys., 430, 905-910 (2005)
	Exploratory C star search in the disk of M 31 beyond 30 kpc.
o	Table 3: <[BD2005] NN> (Nos 1-15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BD2006]
[BD2006]	(Battinelli+Demers, 2006)
Write:	<<[BD2006] NN>>
N:	47
Object:	C* (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Note:	TNG observations of N=47 carbon stars in DDO 190.
in source:	DDO 190
Ref:	=2006A&A...447..473B
by	BATTINELLI P. , DEMERS S.
	Astron. Astrophys., 447, 473-480 (2006)
	The C star population of DDO 190.
o	Table 2: <[BD2006] NN> (Nos 1-47).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BD2008]
[BD2008]	(Blakeslee+DeGraaff, 2008)
Write:	<<[BD2008] NNNN>>
N:	40
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations of the field of ESO 325-004 field in the cluster ACO S 740.
in source:	ACO S 740
Ref:	=2008AJ....136.2295B
by	BLAKESLEE J.P. , BARBER DEGRAAFF R.
	Astron. J., 136, 2295-2305 (2008)
	Ultra-compact dwarf candidates near the lensing galaxy in Abell S0740.
o	Table 1: <[BD2008] NNNN> N=40 among (Nos 211-5503).
=E=	Catalogue in electronic form as <J/AJ/136/2295/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BD2011]
[BD2011]	(Battinelli+Demers, 2011)
Write:	<<[BD2011] NNN>>
N:	33+31
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	CTIO 1.5m telescope CPAPIR (NIR) and Mont Megantic 1.6m telescope observations of N=33 cyclic variables (Nos 1-33) and N=31 semi-regular and irregular variables (Nos 100-130).
in source:	NGC 6822
Ref:	=2011A&A...525A..69B
by	BATTINELLI P. , DEMERS S.
	Astron. Astrophys., 525A, 69-69 (2011)
	Long period variable survey in NGC 6822.
o	Tables 3-4: <[BD2011] NNN> (Nos 1-33, 100-130).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BD2013]
[BD2013]	(Battinelli+Demers, 2013)
Write:	<<[BD2013] Sgr-NNa>>
N:	29
Object:	C* + V* (SIMBAD class: C* = Carbon Star)
Note:	La Silla 60cm telescope REMIR and ROSS observations of N=29 carbon stars in the Sagittarius dwarf spheroidal galaxy.
in source:	NAME Sgr Dwarf Galaxy = NAME Sgr dSph
Ref:	=2013A&A...553A..93B
by	BATTINELLI P. , DEMERS S.
	Astron. Astrophys., 553A, 93-93 (2013)
	The variability of carbon stars in the Sagittarius dwarf spheroidal galaxy.
o	Table 1: <[BD2013] Sgr-NNa> N=29 (Nos 1-26, 13a, 15a, 23a).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BDA
BDA	(Blum+Davis, field A)
Write:	<<BDA NN A>>
N:	10
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Radio in field 'A'. See also BDB
Ref:	=1968ApL.....2...41B
by	BLUM E.J. , DAVIS M.M.
	Astrophys. Lett., 2, 41-44 (1968)
	Spectral characteristics of radio sources from a limited survey at 6cm.
o	Table I: <BDA NN A> (Nos 1-10). Table II: <BDB NN B> (Nos 1-24).
Details on Acronym: [BDA2008]
[BDA2008]	(Boue+Durret+Adami+, 2008)
Write:	<<[BDA2008] ACO85JHHMMSS.ss+DDMMSS.s>>
N:	101+6
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	CFHT MegaPrime-MegaCam and ESO 2.2m WFI observations.
in source:	ACO 85
Ref:	=2008A&A...489...11B
by	BOUE G. , DURRET F., ADAMI C., MAMON G.A., ILBERT O., CAYATTE V.
	Astron. Astrophys., 489, 11-22 (2008)
	An optical view of the filament region of Abell 85.
o	Tables A4, A5, col(1): numbering NNN is not used in SIMBAD.
o	Tables A4, A5, col(2): <[BDA2008] ACO85JHHMMSS.ss+DDMMSS.s> N=101+6.
=E=	Catalogue in electronic form as J/A+A/489/11
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BDB
BDB	(Blum+Davis, field B)
Write:	<<BDB NN B>>
N:	24
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Radio in field 'B'. See also BDA
Ref:	=1968ApL.....2...41B
by	BLUM E.J. , DAVIS M.M.
	Astrophys. Lett., 2, 41-44 (1968)
	Spectral characteristics of radio sources from a limited survey at 6cm.
o	Table I: <BDA NN A> (Nos 1-10). Table II: <BDB NN B> (Nos 1-24).
Details on Acronym: [BDB2003]
[BDB2003]	(Bica+Dutra+Barbuy, 2003)
Write:	<<[BDB2003] GLLL.ll+BB.bb>>
N:	275
Object:	IR Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	Compilation of infrared star clusters in the Galaxy.
Ref:	=2003A&A...397..177B
by	BICA E. , DUTRA C.M., BARBUY B.
	Astron. Astrophys., 397, 177-180 (2003)
	A Catalogue of infrared star clusters and stellar groups.
o	Table 1: for IC 348 and subclusters IC 348a to i, the 2000 coordinates do not correspond to the galactic coordinates, so a second format 'GLLL.ll+BB.bb' is created for each cluster.
o	Table 1: <[BDB2003] GLLL.ll+BB.bb> N=276.
=E=	Catalogue in electronic form as J/A+A/397/177
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDB2006]
[BDB2006]	(Butt+Drake+Benaglia+, 2006)
Write:	<<[BDB2006] NNN>>
N:	240
Object:	(x) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of TeV J2032+4130.
in source:	TeV J2032+4130
Ref:	=2006ApJ...643..238B
by	BUTT Y.M. , DRAKE J., BENAGLIA P., COMBI J.A., DAME T., MINIATI F., ROMERO G.E.
	Astrophys. J., 643, 238-244 (2006)
	Deeper Chandra follow-up of Cygnus TeV source perpetuates mystery.
o	Table 1: <[BDB2006] NNN> (Nos 1-240).
=E=	Catalogue in electronic form as J/ApJ/643/238
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDB2007]
[BDB2007]	(Boquiem+Duc+Braine+, 2007)= (GALEX)
Write:	<<[BDB2007] NN>> <<[BDB2007] GALEX JHHMMSS.ss+DDMMSS.ss>>
N:	32
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	UV GALEX observations of NGC 5291, combined with archival Spitzer Space Telescope data and VLA HI data.
in source:	NGC 5291
Ref:	=2007A&A...467...93B
by	BOQUIEN M. , DUC P.-A., BRAINE J., BRINKS E., LISENFELD U., CHARMANDARIS V.
	Astron. Astrophys., 467, 93-106 (2007)
	Polychromatic view of intergalactic star formation in NGC 5291.
o	Fig.3, Table 1: <[BDB2007] NN> (Nos 1-29) = <[BDB2007] GALEX JHHMMSS.ss+DDMMSS.ss> N=32.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDB2009]
[BDB2009]	(Bussmann+Dey+Borys+, 2009)
Write:	<<[BDB2009] SNN>>
N:	12
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	SHARC-II (350mu.m) and CARMA (1mm) observations of N=12 Dust-Obscured Galaxies (DOGs) in the Bootes field of the NOAO Deep Wide-Field Survey.
in source:	NAME Bootes Field
Ref:	=2009ApJ...705..184B
by	BUSSMANN R.S. , DEY A., BORYS C., DESAI V., JANNUZI B.T., LE FLOC'H E., MELBOURNE J., SHETH K., SOIFER B.T.
	Astrophys. J., 705, 184-198 (2009)
	Infrared luminosities and dust properties of z ~ 2 dust-obscured galaxies.
o	Table 1: <[BDB2009] SNN> (Nos S1-S12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDB2015]
[BDB2015]	(Bechtol+Drlica-Wagner+Balbinot+, 2015)
Write:	<<[BDB2015] DES JHHMM.m+DDMM>>
N:	8
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=8 Milky Way satellite galaxy candidates, using optical imaging data collected during the first year of the Dark Energy Survey (DES).
Ref:	=2015ApJ...807...50B
by	BECHTOL K. , DRLICA-WAGNER A., BALBINOT E., PIERES A., SIMON J.D., YANNY B., SANTIAGO B., WECHSLER R.H., FRIEMAN J., WALKER A.R., WILLIAMS P., ROZO E., RYKOFF E.S., QUEIROZ A., LUQUE E., BENOIT-LEVY A., TUCKER D., SEVILLA I., GRUENDL R.A., DA COSTA L.N., FAUSTI NETO A., MAIA M.A.G., ABBOTT T., ALLAM S., ARMSTRONG R., BAUER A.H., BERNSTEIN G.M., BERNSTEIN R.A., BERTIN E., BROOKS D., BUCKLEY-GEER E., BURKE D.L., CARNERO ROSELL A., CASTANDER F.J., COVARRUBIAS R., D'ANDREA C.B., DEPOY D.L., DESAI S., DIEHL H.T., EIFLER T.F., ESTRADA J., EVRARD A.E., FERNANDEZ E., FINLEY D.A., FLAUGHER B., GAZTANAGA E., GERDES D., GIRARDI L., GLADDERS M., GRUEN D., GUTIERREZ G., HAO J., HONSCHEID K., JAIN B., JAMES D., KENT S., KRON R., KUEHN K., KUROPATKIN N., LAHAV O., LI T.S., LIN H., MAKLER M., MARCH M., MARSHALL J., MARTINI P., MERRITT K.W., MILLER C., MIQUEL R., MOHR J., NEILSEN E., NICHOL R., NORD B., OGANDO R., PEOPLES J., PETRAVICK D., PLAZAS A.A., ROMER A.K., ROODMAN A., SAKO M., SANCHEZ E., SCARPINE V., SCHUBNELL M., SMITH R.C., SOARES-SANTOS M., SOBREIRA F., SUCHYTA E., SWANSON M.E.C., TARLE G., THALER J., THOMAS D., WESTER W., ZUNTZ J., (The DES Collaboration)
	Astrophys. J., 807, 50 (2015)
	Eight new Milky Way companions discovered in first-year dark energy survey data.
o	Table 1: <[BDB2015] DES JHHMM.m+DDMM> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDB2017]
[BDB2017]	(Barrett+Dieck+Beasley+, 2017)
Write:	<<[BDB2017] CCC N>>
N:	20
Object:	Catacl. V* (SIMBAD class: CataclyV* = Cataclysmic Binary)
Note:	Jansky VLA C- X- K- and Q-bands observations of N=20 magnetic cataclysmic variables (MCVs).
Ref:	=2017AJ....154..252B
by	BARRETT P.E. , DIECK C., BEASLEY A.J., SINGH K.P., MASON P.A.
	Astron. J., 154, 252-252 (2017)
	A Jansky VLA survey of magnetic cataclysmic variable stars. I. The data.
o	Table 2: <[BDB2017] CCC N> N=20.
=E=	Catalogue in electronic form as <J/AJ/154/252/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDB95]
[BDB95]	(Bird+Davis+Beers, 1995)
Write:	<<[BDB95] A2151C>> <<[BDB95] A2151W>>
N:	3
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observation of ACO 2151.
in source:	ACO 2151
Ref:	=1995AJ....109..920B
by	BIRD C.M. , DAVIS D.S., BEERS T.C.
	Astron. J., 109, 920-927 (1995)
	Subcluster mergers and galaxy infall in A 2151.
o	Table 2: <[BDB95] A2151C>, <[BDB95] A2151W> (Nos N, E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDC2001]
[BDC2001]	(Blum+Damineli+Conti, 2001)
Write:	<<[BDC2001] W31-NNN>>
N:	251
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=16 stars in Gal 10.2-0.3, an HII region in W 31. See also [BDC99], [BCD2000], FBDDC
in source:	W 31:GAL 10.2-0.3:NAME Star Cluster in GAL 10.2-0.3 = NAME Star Cluster in GAL 10.2-0.3
Ref:	=2001AJ....121.3149B
by	BLUM R.D. , DAMINELI A., CONTI P.S.
	Astron. J., 121, 3149-3159 (2001)
	The stellar content of obscured galactic giant H II regions. III. W31.
o	Par. 3, Fig.1a: the bright object 'A' is USNO-A2.0 0675-24273097
o	Tables 1, 2, 3: <[BDC2001] W31-NNN> N=16 among (Nos 1-251).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDC2005]
[BDC2005]	(Bloom+Dupree+Chen+, 2005)
Write:	<<[BDC2005] A>>
N:	4
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	MIKE (Magellan II/Clay) guider CCD camera observations. N=4 sources in the field of GRB 050724.
Ref:	=2005GCN..3672....1B
by	BLOOM J.S. , DUPREE A., CHEN H.-W., PROCHASKA J.X.
	GRB Coordinates Network, Circular Service, 3672, 1-None (2005)
	GRB 050724: optical imaging/astronomy.
o	<[BDC2005] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDC2012]
[BDC2012]	(Bruce+Dunlop+Cirasuolo+, 2012)
Write:	<<[BDC2012] NNNNNN>>
N:	215
Object:	G (SIMBAD class: Galaxy)
Note:	N=215 galaxies in the UKIDSS Deep Survey (UDS) field. Use of HST WFC3 imaging, as part of the CANDELS multi-cycle treasury programme.
Ref:	=2012MNRAS.427.1666B
by	BRUCE V.A. , DUNLOP J.S., CIRASUOLO M., McLURE R.J., TARGETT T.A., BELL E.F., CROTON D.J., DEKEL A., FABER S.M., FERGUSON H.C., GROGIN N.A., KOCEVSKI D.D., KOEKEMOER A.M., KOO D.C., LAI K., LOTZ J.M., McGRATH E.J., NEWMAN J.A., VAN DER WEL A.
	Mon. Not. R. Astron. Soc., 427, 1666-1701 (2012)
	The morphologies of massive galaxies at 1 < z < 3 in the CANDELS-UDS field: compact bulges, and the rise and fall of massive discs.
o	Tables D1-D2: <[BDC2012] NNNNNN> N=215 among (Nos 100222-123457).
=E=	Catalogue in electronic form as J/MNRAS/427/1666
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDC2016]
[BDC2016]	(Burkhardt+Dollhopf+Corby+, 2016) (Not yet in Simbad)
Write:	<<[BDC2016] BNa>>
N:	3
Object:	Clump (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	CARMA observations of the southern portion of the LDN 1157 outflow. See also [TB95].
in source:	LDN 1157: [DE95] LDN 1157 B1 = [DE95] LDN 1157 B1
Ref:	=2016ApJ...827...21B
by	BURKHARDT A.M. , DOLLHOPF N.M., CORBY J.F., CARROLL P.B., SHINGLEDECKER C.N., LOOMIS R.A., BOOTH S.T., BLAKE G.A., HERBST E., REMIJAN A.J., McGUIRE B.A.
	Astrophys. J., 827, 21-21 (2016)
	CSO and CARMA observations of L1157. II. Chemical complexity in the shocked outflow.
o	Fig. 2, Table 2: <[BDC2016] BNa> (Nos B0k-B0l, B2d).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDC99]
[BDC99]	(Blum+Damineli+Conti, 1999)
Write:	<<[BDC99] W43 Cluster>> <<[BDC99] W43 N>>
N:	1+3
Object:	Cluster of * + *inCl (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=1 Cl* in W 43 complex, and N=3 brightest members of this cluster. See also [BCD2000], [BDC2001], FBDDC
in source:	W 43
Ref:	=1999AJ....117.1392B
by	BLUM R.D. , DAMINELI A., CONTI P.S.
	Astron. J., 117, 1392-1401 (1999)
	The stellar content of obscured galactic giant H II regions. I. W43.
o	Par. 3.1.1., M 1 misprint for M 17. Par. 4.3: G30.8N and G30.8S = [LDW85] 30.8N and 30.8S.
o	Fig.1: <[BDC99] W43 Cluster> N=1, <[BDC99] W43 N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDD2007]
[BDD2007]	(Brand+Dey+Desai+, 2007)= (SST24)
Write:	<<[BDD2007] SST24 JHHMMSS.s+DDMMSS>> <<[BDD2007] JHHMMSS.s+DDMMSS>> (not recognised by Simbad, but found in literature)
N:	10
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck NIRSPEC and Gemini NIRI observations of faint ultraluminous IR galaxies from the Spitzer Bootes survey. using Keck NIRSPEC and GGemini NIRI.
Ref:	=2007ApJ...663..204B
by	BRAND K. , DEY A., DESAI V., SOIFER B.T., BIAN C., ARMUS L., BROWN M.J.I., LE FLOC'H E., HIGDON S.J., HOUCK J.R., JANNUZI B.T., WEEDMAN D.W.
	Astrophys. J., 663, 204-217 (2007)
	Optical line diagnostics of z ~ 2 optically faint ultraluminous infrared galaxies in the Spitzer Bootes survey.
o	Table 1: <[BDD2007] SST24 JHHMMSS.s+DDMMSS> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDD2008]
[BDD2008]	(Buyle+De Rijcke+Debattista+, 2008)
Write:	<<[BDD2008] JHHMMSS.ss+DDMMSS.ss>>
N:	1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLT 8.6GHz observations of VCC 128.
in source:	VCC 128
Ref:	=2008ApJ...685..915B
by	BUYLE P. , DE RIJCKE S., DEBATTISTA V.P., FERRERAS I., PASQUALI A., SETH A., MORELLI L.
	Astrophys. J., 685, 915-918 (2008)
	Radio continuum observations of the candidate supermassive black hole in the dwarf elliptical VCC 128.
o	Fig.1, text: <[BDD2008] JHHMMSS.ss+DDMMSS.ss> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BDF
BDF	(BIMA Deep Field)
*****	Avoid the usage of BDF, prefer [HCG2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BDF2018]
[BDF2018]	(Becker+Davies+Furlanetto+, 2018)
Write:	<<[BDF2018] JHHMMSS+DDMMSS>>
N:	806
Object:	Poss. LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Subaru Hyper Suprime-Cam observations of N=806 LAE candidates in the field of the z=6.0 quasar ULAS J014837.63+060020.0.
Ref:	=2018ApJ...863...92B
by	BECKER G.D. , DAVIES F.B., FURLANETTO S.R., MALKAN M.A., BOERA E., DOUGLASS C.
	Astrophys. J., 863, 92-92 (2018)
	Evidence for large-scale fluctuations in the metagalactic ionizing background near redshift six.
o	Table 2: <[BDF2018] JHHMMSS+DDMMSS> N=806.
=E=	Catalogue in electronic form as <J/ApJ/863/92/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDF99]
[BDF99]	(Beaulieu+Dopita+Freeman, 1999)
Write:	<<[BDF99] SBNN>>
N:	56
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	N=56 PN from S. Beaulieu Thesis (1996) PN SB.
Ref:	=1999ApJ...515..610B
by	BEAULIEU S.F. , DOPITA M.A., FREEMAN K.C.
	Astrophys. J., 515, 610-632 (1999)
	A survey of planetary nebulae in the southern Galactic Bulge.
o	Table 8: <[BDF99] SBNN> (Nos SB1 to SB56).
=E=	Catalogue in electronic form as J/ApJ/515/610
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDG98]
[BDG98]	(Barton+De Carvalho+Geller, 1998)
Write:	<<[BDG98] JHHMMSS.s+DDMMSS>>
N:	509
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=509 galaxies in 14 RSCG clusters
Ref:	=1998AJ....116.1573B
by	BARTON E.J. , DE CARVALHO R.R., GELLER M.J.
	Astron. J., 116, 1573-1590 (1998)
	Environments of redshift survey compact groups of galaxies.
o	Table 3: <[BDG98] JHHMMSS.s+DDMMSS> N=509.
=E=	Catalogue in electronic form as J/AJ/116/1573
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDH2007]
[BDH2007]	(Broderick+De Breuck+Hunstead+, 2007)
Write:	<<[BDH2007] B0529-549 W>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA observations of PKS B0529-549: N=2 components.
in source:	PKS 0529-549
Ref:	=2007MNRAS.375.1059B
by	BRODERICK J.W. , DE BREUCK C., HUNSTEAD R.W., SEYMOUR N.
	Mon. Not. R. Astron. Soc., 375, 1059-1069 (2007)
	An extreme rotation measure in the high-redshift radio galaxy PKS B0529-549.
o	Table 2, Fig.1: <[BDH2007] B0529-549 W> (Nos W, E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDH2018]
[BDH2018]	(Barrado+De Gregorio Monsalvo+Huelamo+, 2018)
Write:	<<[BDH2018] B30-LBNN a>>
N:	34+224
Object:	(smm) + * (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	APEX LABOCA 870µm and and CAHA Omega2000 NIR observations of N=34 submillimeter sources and N=224 very low-mass stars and brown dwarfs in the Barnard 30 dark cloud. Use of archival Spitzer IRAC and MIPS data.
in source:	Barnard 30
Ref:	=2018A&A...612A..79B
by	BARRADO D. , DE GREGORIO MONSALVO I., HUELAMO N., MORALES-CALDERON M., BAYO A., PALAU A., RUIZ M.T., RIVIERE-MARICHALAR P., BOUY H., MORATA O., STAUFFER J.R., EIROA C., NORIEGA-CRESPO A.
	Astron. Astrophys., 612A, 79-79 (2018)
	Early phases in the stellar and substellar formation and evolution. Infrared and submillimeter data in the Barnard 30 dark cloud.
o	Table 2: <[BDH2018] B30-LBNN> (Nos 1-34). Table 3: <[BDH2018] B30-LBNN a> N=224 among (Nos LB01 a to LB33 a).
=E=	Catalogue in electronic form as J/A+A/612/A79
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDH96]
[BDH96]	(Benitez+Dultzin-Hacyan+Heidt+, 1996)
Write:	<<[BDH96] A>>
N:	11
Object:	Nebula (SIMBAD class: ISM = Interstellar Medium Object)
Stat:	is completely incorporated in Simbad
Note:	(Nos A-K), Nebulosities surrounding Ohio J 287 Map See also [YJI97]
Ref:	=1996ApJ...464L..47B
by	BENITEZ E. , DULTZIN-HACYAN D., HEIDT J., SILLANPAEAE A., NILSSON K., PURSIMO T., TEERIKORPI P., TAKALO L.O.
	Astrophys. J., 464, 47-50 (1996)
	The close environment of OJ 287: underlying nebulosity and a possible optical jet?
o	Table 1: <[BDH96] A> (Nos A-H).
Ref:	=1997ApJ...484L.113Y
by	YANNY B. , JANNUZI B.T., IMPEY C.
	Astrophys. J., 484, 113-116 (1997)
	Hubble Space Telescope imaging of the BL Lacertae object OJ 287.
o	Gh is a ghost image, not in SIMBAD
o	Table 1: <[BDH96] A> (Nos I-K) added. Table 1: <[YJI97] Ext>, <[YJI97] SW>, <[YJI97] Gh>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDI2019]
[BDI2019]	(Benaglia+del Palacio+Ishwara-Chandra+, 2019) (Not yet in Simbad)
Write:	<<[BDI2019] GNNN-NNN>> <<[BDI2019] INN>>
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	GMRT observations at 150, 325, and 610MHz of N=700 radio sources, N=53 of which are found at more than one band (format INN).
Ref:	=2019A&A...625A..99B
by	BENAGLIA P. , DEL PALACIO S., ISHWARA-CHANDRA C.H., DE BECKER M., ISEQUILLA N.L., SAPONARA J.
	Astron. Astrophys., 625A, 99-99 (2019)
	Investigation of the WR 11 field at decimeter wavelengths.
o	Table 4: <[BDI2019] GNNN-NNN> (Nos G150-1 to G150-410, G325-1 to G325-224, G610-1 to G610-66). Table 5: <[BDI2019] INN> (Nos I01-I53).
=E=	Catalogue in electronic form as <J/A+A/625/A99/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDJ2005]
[BDJ2005]	(Barr+Davies+Jorgensen+, 2005)
Write:	<<[BDJ2005] NNNN>>
N:	43
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Gemini Multi-Object Spectrograph on GMOS-N imaging and spectroscopy of the cluster RX J0142.0+2131.
in source:	RX J0142.0+2131
Ref:	=2005AJ....130..445B
by	BARR J. , DAVIES R., JORGENSEN I., BERGMANN M., CRAMPTON D.
	Astron. J., 130, 445-474 (2005)
	RX J0142.0+2131. I. The galaxy content of an X-ray-luminous galaxy cluster at z=0.28.
o	Fig.2, Table 7: <[BDJ2005] NNNN> N=43 among (Nos 1-1472).
=E=	Catalogue in electronic form as J/AJ/130/445
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDK87]
[BDK87]	(Bergeron+D'Odorico+Kunth, 1987)
Write:	<<[BDK87] NN>>
N:	46
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Objects around PKS 1327-206 Map in Fig. 8 See also [B86b], [BB86b], [B88], [BBK88], [BB91], [BCS92], [GB97]
Ref:	=1987A&A...180....1B
by	BERGERON J. , D'ODORICO S., KUNTH D.
	Astron. Astrophys., 180, 1-11 (1987)
	Comprehensive study of the QSO-galaxy pair 1327-206 and the extent of low ionization galactic haloes.
o	Table 4: <[BDK87] NN> (Nos 1-46)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDL2001]
[BDL2001]	(Braine+Duc+Lisenfeld+, 2001)= (TDG)
Write:	<<[BDL2001] NGC NNNNW>> <<[BDL2001] IC NNNNW>>
N:	8
Object:	Tidal dwarf G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=8 tidal dwarf galaxies related to an NGC NNNN or IC NNNN system. See also [BLD2000].
in source:	NGC 7252
in source:	NGC 4038
in source:	NGC 4676
in source:	NGC 5291
in source:	NGC 7319
in source:	NGC 2782
in source:	IC 1182 = Mrk 298
Ref:	=2001A&A...378...51B
by	BRAINE J. , DUC P.-A., LISENFELD U., CHARMANDARIS V., VALLEJO O., LEON S., BRINKS E.
	Astron. Astrophys., 378, 51-69 (2001)
	Abundant molecular gas in tidal dwarf galaxies: On-going galaxy formation.
o	in ref list Combes, Dupraz 1988A&A...203L...9C instead of 203.9. Table 2: Arp 105S = [BLD2000] A105S, Arp 245N = [BLD2000] A245N.
o	Table 1: <[BDL2001] NGC NNNNW> N=7, <[BDL2001] IC 1182E> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDL2003]
[BDL2003]	(Battinelli+Demers+Letarte, 2003)
Write:	<<[BDL2003] NN>>
N:	25
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Note:	CFH12K observations. Search for carbon stars in the outer disk of M 31. See also [ADK2000], [BD2000], [DB2002], [LDB2002], [DBL2003], [DBL2003b], [BD2004a], [BD2004b], [DBL2004].
in source:	M 31 = NGC 224
Ref:	=2003AJ....125.1298B
by	BATTINELLI P. , DEMERS S., LETARTE B.
	Astron. J., 125, 1298-1308 (2003)
	Carbon star survey in the Local Group. V. The outer disk of M 31.
o	Table 3: <[BDL2003] NN> (Nos 1-25).
=E=	Catalogue in electronic form as J/AJ/125/1298
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDL2009]
[BDL2009]	(Bussmann+Dey+Lotz+, 2009)= (SST24) = (DOG)
Write:	<<[BDL2009] NN>> <<[BDL2009] SST24 JHHMMSS.s+DDMMSS>>
N:	31
Object:	G (SIMBAD class: Galaxy)
Note:	HST ACS, WFPC2, and NICMOS observations of N=31 24mu.m bright z about 2 dust obscured galaxies.
Ref:	=2009ApJ...693..750B
by	BUSSMANN R.S. , DEY A., LOTZ J., ARMUS L., BRAND K., BROWN M.J.I., DESAI V., EISENHARDT P., HIGDON J., HIGDON S., JANNUZI B.T., LE FLOC'H E., MELBOURNE J., SOIFER B.T., WEEDMAN D.
	Astrophys. J., 693, 750-770 (2009)
	Hubble Space Telescope morphologies of z ~ 2 dust obscured galaxies. I. Power-law sources.
o	STT24 J142538.0+332607 is a misprint for STT24 J142538.2+351855.
o	Tables 1-6: <[BDL2009] NN> (Nos 1-31) = <[BDL2009] SST24 JHHMMSS.s+DDMMSS> N=31.
Details on Acronym: BDM
BDM	(Baart+De Jager+Mountfort)
*****	Avoid the usage of BDM, prefer BJM
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDM2001]
[BDM2001]	(Boumis+Dickinson+Meaburn+, 2001)
Write:	<<[BDM2001] Arc A>>
N:	2
Object:	Arc (SIMBAD class: ISM = Interstellar Medium Object)
Stat:	is completely incorporated in Simbad
Note:	Deep Halpha observations with the Manchester Wide Field Camera and the Kryonerion Observatory, Greece.
in source:	NAME Eri Region
Ref:	=2001MNRAS.320...61B
by	BOUMIS P. , DICKINSON C., MEABURN J., GOUDIS C.D., CHRISTOPOULOU P.E., LOPEZ J.A., BRYCE M., REDMAN M.P.
	Mon. Not. R. Astron. Soc., 320, 61-65 (2001)
	Deep Hα imagery of the Eridanus shells.
o	Fig.3: <[BDM2001] Arc A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDM2004]
[BDM2004]	(Bregman+Dupke+Miller, 2004)
Write:	<<[BDM2004] QSO J0057-2222 abs N.NNNN>>
N:	3
Object:	Absorber
Note:	FUSE observations. N=3 absorption systems in Ton S 180 = QSO J0057-2222.
Ref:	=2004ApJ...614...31B
by	BREGMAN J.N. , DUPKE R.A., MILLER E.D.
	Astrophys. J., 614, 31-36 (2004)
	Cosmic filaments in superclusters.
o	Text, Fig.3: <[BDM2004] QSO J0057-2222 abs N.NNNN> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDM2012]
[BDM2012]	(Bowler+Dunlop+Mclure+, 2012)
Write:	<<[BDM2012] NNNNNN>>
N:	10+34
Object:	Poss. G (SIMBAD class: Galaxy_Candidate = Galaxy Candidate)
Note:	z>6.5 galaxy candidates in the near-infrared UltraVISTA imaging of the COSMOS field.
in source:	NAME COSMOS Field
Ref:	=2012MNRAS.426.2772B
by	BOWLER R.A.A. , DUNLOP J.S., McLURE R.J., McCRACKEN H.J., MILVANG-JENSEN B., FURUSAWA H., FYNBO J.P.U., LE FEVRE O., HOLT J., IDEUE Y., IHARA Y., ROGERS A.B., TANIGUCHI Y.
	Mon. Not. R. Astron. Soc., 426, 2772-2788 (2012)
	Discovery of bright z ≃ 7 galaxies in the UltraVISTA survey.
o	Tables 2-3: <[BDM2012] NNNNNN> N=10 among (Nos 2233-277912).
Ref:	=2014MNRAS.440.2810B
by	BOWLER R.A.A. , DUNLOP J.S., McLURE R.J., ROGERS A.B., McCRACKEN H.J., MILVANG-JENSEN B., FURUSAWA H., FYNBO J.P.U., TANIGUCHI Y., AFONSO J., BREMER M.N., LE FEVRE O.
	Mon. Not. R. Astron. Soc., 440, 2810-2842 (2014)
	The bright end of the galaxy luminosity function at z ≃ 7: before the onset of mass quenching ?
o	Tables 2-4: <[BDM2012] NNNNNN> N=34 among (Nos 2103-583226).
=E=	Catalogue in electronic form as <J/MNRAS/440/2810/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDM2015]
[BDM2015]	(Bowler+Dunlop+McLure+, 2015) (Not yet in Simbad)
Write:	<<[BDM2015] SNN>>
N:	47
Object:	Poss. High redshift G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=47 candidate high-redshift galaxies selected from the deep Subaru z'-band imaging in the UltraVISTA/COSMOS and UDS/SXDS fields.
Ref:	=2015MNRAS.452.1817B
by	BOWLER R.A.A. , DUNLOP J.S., McLURE R.J., McCRACKEN H.J., MILVANG-JENSEN B., FURUSAWA H., TANIGUCHI Y., LE FEVRE O., FYNBO J.P.U., JARVIS M.J., HAUSSLER B.
	Mon. Not. R. Astron. Soc., 452, 1817-1840 (2015)
	The galaxy luminosity function at z~= 6 and evidence for rapid evolution in the bright end from z~=7 to 5.
o	Table B1: <[BDM2015] SNN> (Nos S1-S47).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BDN
BDN	(Bernes, Dark Neb)
Object:	HII + RFN (SIMBAD class: GalNeb = Nebula)
Ref:	=1977A&AS...29...65B
by	BERNES C.
	Astron. Astrophys., Suppl. Ser., 29, 65-70 (1977)
	A catalogue of bright nebulosities in opaque dust clouds.
o	Catalogue: <[B77] NNN> (Nos 1-160)
*****	Avoid the usage of BDN, prefer [B77]
Origin	of the Acronym: L (2002A&A...383..631D)
Details on Acronym: BDN
BDN	(Bright Dark Nebula)
N:	1
Object:	Bright-Dark Nebula (SIMBAD class: DarkNeb = Dark Cloud (nebula))
Ref:	=1974A&A....32..465F
by	FITZGERALD M.P.
	Astron. Astrophys., 32, 465-474 (1974)
	A remarkable "Bright Dark Nebula" in Chamaeleon.
o	<NAME BDN> <NAME CDN>
Details on Acronym: [BDP2014]
[BDP2014]	(Beccari+De Marchi+Panagia+, 2014)= ([BDP2014a])
Write:	<<[BDP2014] NN>>
N:	59
Object:	H-alpha Em* (SIMBAD class: EmLine* = Emission-line Star)
Note:	N=59 Hα excess emission stars in 47 Tuc. Use of HST ACS archival observations.
in source:	NGC 104 = 47 Tuc
Ref:	=2014MNRAS.437.2621B
by	BECCARI G. , DE MARCHI G., PANAGIA N., PASQUINI L.
	Mon. Not. R. Astron. Soc., 437, 2621-2631 (2014)
	Hα photometry of low-mass stars in 47 Tucanae: chromospheric activity and exotica.
o	Table 2: <[BDP2014] NN> (Nos 1-59).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDP2014a]
[BDP2014a]	(Beccari+De Marchi+Panagia+, 2014) (Not yet in Simbad)
*****	Avoid the usage of [BDP2014a], prefer [BDP2014]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDP2014b]
[BDP2014b]	(Baxter+Dobbie+Parker+, 2014)
Write:	<<[BDP2014b] CDDSNN>>
N:	53
Object:	(SIMBAD class: = Double or Multiple Star)
Stat:	is completely incorporated in Simbad
Note:	WHT ISIS, VLT FORS2, Gemini-North and -South GMOS, GTC OSIRIS spectroscopy of N=53 candidate double-degenerate systems (CDDS). Use of SDSS DR7 data.
Ref:	=2014MNRAS.440.3184B
by	BAXTER R.B. , DOBBIE P.D., PARKER Q.A., CASEWELL S.L., LODIEU N., BURLEIGH M.R., LAWRIE K.A., KULEBI B., KOESTER D., HOLLAND B.R.
	Mon. Not. R. Astron. Soc., 440, 3184-3201 (2014)
	Component masses of young, wide, non-magnetic white dwarf binaries in the Sloan Digital Sky Survey Data Release 7.
o	Table 1: <[BDP2014b] CDDSNN> (Nos CDDS1-CDDS53).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDR2011]
[BDR2011]	(Brown+Duesterhoeft+Rudnick+, 2011)
Write:	<<[BDR2011] JHHMM+DD>> <<[BDR2011] HHMM+DD>> (not recognised by Simbad, but found in literature)
N:	1
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	VLA observations at 1.4 and 0.3GHz of a radio-selected cluster of galaxies.
Ref:	=2011ApJ...727L..25B
by	BROWN S. , DUESTERHOEFT J., RUDNICK L.
	Astrophys. J., 727L, 25 (2011)
	Multiple shock structures in a radio-selected cluster of galaxies.
o	Text: <[BDR2011] J0217+70> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BDS
BDS	(Burnham, Double *)= (BGC)
Write:	<<BDS NNNNNAA>>
N:	13665
Object:	(SIMBAD class: = Double or Multiple Star)
Note:	Superseded by Aitken's New General Catalogue: ADS, and by IDS nomenclature.
Ref:	=1906BDS...C......0B
by	BURNHAM S.W.
	Burnham Double Star, 0-None (1906)
	A general catalogue of double stars within 121° of the North Pole.
o	<BDS NNNNNAA> N=13665.
Details on Acronym: BDS
BDS	(Bird+Dickey+Salpeter)
*****	Avoid the usage of BDS, prefer [BDS93]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BDS
BDS	(Blaauw+Danziger+Schuster)
*****	Avoid the usage of BDS, prefer BlDz
Details on Acronym: [BDS2000]
[BDS2000]	(Buckalew+Dufour+Shopbell+, 2000)
Write:	<<[BDS2000] {S\|C\|U}N>>
N:	7+5+3
Object:	* + Cluster of * + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of NGC 1569. N=7 WR* candidates (Nos S1-S7). N=5 Cl* (Nos C1-C5). N=3 sources of unknown origin (Nos U1-U3).
in source:	NGC 1569
Ref:	=2000AJ....120.2402B
by	BUCKALEW B.A. , DUFOUR R.J., SHOPBELL P.L., WALTER D.K.
	Astron. J., 120, 2402-2414 (2000)
	The starburst-interstellar medium interaction in NGC 1569. I. Location and nature of He II sources using Hubble space telescope WFPC2 imagery.
o	Table 2: <[BDS2000] SN> (Nos S1-S7). Table 3: <[BDS2000] CN> (Nos C1-C5). Table 4: <[BDS2000] UN> (Nos U1-U3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDS2003]
[BDS2003]	(Bica+Dutra+Soares+, 2003)
Write:	<<[BDS2003] NNN>>
N:	167
Object:	(IR) Stellar Cluster (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	N=167 new infrared clusters, stellar groups, and candidates. See also Paper I [DBS2003].
Ref:	=2003A&A...404..223B
by	BICA E. , DUTRA C.M., SOARES J., BARBUY B.
	Astron. Astrophys., 404, 223-232 (2003)
	New infrared star clusters in the Northern and Equatorial Milky Way with 2MASS.
o	Table 1 : GM 1-45 = GM 3-45, Gy 3-4 = [G84c] 4 in Simbad.
o	Tables 1, 2: <[BDS2003] NNN> (Nos 1-167).
=E=	Catalogue in electronic form as J/A+A/404/223
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDS93]
[BDS93]	(Bird+Dickey+Salpeter, 1993)= (BDS)
Write:	<<[BDS93] NNN>>
N:	127
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
in source:	ACO 2151
Ref:	=1993ApJ...404...81B
by	BIRD C.M. , DICKEY J.M., SALPETER E.E.
	Astrophys. J., 404, 81-93 (1993)
	Dark matter and dynamics in the Hercules cluster (A 2151).
o	Table 1: HNNN = [D80] ACO 2151 NNN, H1559174 = [BDS93] 32
o	<[BDS93] NNN> N =127
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDV2001]
[BDV2001]	(Briggs+De Bruyn+Vermeulen, 2001) (Not yet in Simbad)
Write:	<<[BDV2001] 3C 196 GN>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Note:	N=2 galaxies, optical candidates for 3C 196.
Ref:	=2001A&A...373..113B
by	BRIGGS F.H. , DE BRUYN A.G., VERMEULEN R.C.
	Astron. Astrophys., 373, 113-121 (2001)
	Cold gas kinematics in an L_{} spiral galaxy at z = 0.437: The nature of* damped Lyman-α absorbers.
o	<[BDV2001] 3C 196 GN> (Nos G1-G2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDV69]
[BDV69]	(Bertaud+Dumortier+Veron+, 1969)
Write:	<<[BDV69] BL Lac A>> <<[BDV69] BL Lac a>>
N:	3+9
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Stars in the field of BL Lac: (Nos A-C) are calibration stars, (Nos a-k) d, i and j missing are in the field of BL Lac. (No. l) is added as No. 9 in the field of BL Lac in ref. 1977AJ.....82..453M. (Nos a-k) are often written A to K in the literature... Map.
Ref:	=1969A&A.....3..436B
by	BERTAUD C. , DUMORTIER B., VERON P., WLERICK G., ADAM G., BIGAY J., GARNIER R., DURUY M.
	Astron. Astrophys., 3, 436-442 (1969)
	Etude photometrique et radioelectrique de BL Lac.
o	Fig.1: <[BDV69] BL Lac A> (Nos A-C). Fig.1, Table 1: <[BDV69] BL Lac a> N=8 among (Nos a-k).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDW2002]
[BDW2002]	(Bechtold+Dobrzycki+Wilden+, 2002)
Write:	<<[BDW2002] qHHMM+DDMMa>>
N:	334
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	QSOs observed with FOS/HST.
Ref:	=2002ApJS..140..143B
by	BECHTOLD J. , DOBRZYCKI A., WILDEN B., MORITA M., SCOTT J., DOBRZYCKA D., TRAN K.-V., ALDCROFT T.L.
	Astrophys. J., Suppl. Ser., 140, 143-238 (2002)
	A uniform analysis of the Lyα forest at z = 0-5. III. Hubble Space Telescope faint object spectrograph spectral atlas.
o	Table 1: <[BDW2002] qHHMM+DDMMa> N=334.
=E=	Catalogue in electronic form as J/ApJS/140/143
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDW2009]
[BDW2009]	(Boquien+Duc+Wu+, 2009) (Not yet in Simbad)
Write:	<<[BDW2009] Arp NNN N>> <<[BDW2009] NGC NNNN NN>> <<[BDW2009] SQ NN>> <<[BDW2009] VCC 2062 1>>
N:	6+4+29+4+17+1
Object:	Star Forming Region (SIMBAD class: PartofG = Part of a Galaxy)
Note:	GALEX, CFHT, La Silla (NTT, 3.6m), KPNO, Calar Alto observations of N=61 star-forming regions in six interacting systems. Use of Spitzer data.
in source:	APG 105
in source:	APG 245
in source:	NGC 5291
in source:	NGC 7252
in source:	Stephan's Quintet = HCG 92
in source:	VCC 2062
Ref:	=2009AJ....137.4561B
by	BOQUIEN M. , DUC P.-A., WU Y., CHARMANDARIS V., LISENFELD U., BRAINE J., BRINKS E., IGLESIAS-PARAMO J., XU C.K.
	Astron. J., 137, 4561-4576 (2009)
	Collisional debris as laboratories to study star formation.
o	Figs 1-2, Tables 6-7: <[BDW2009] Arp NNN N> N=6+4. Figs 3-4, Tables 8-9: <[BDW2009] NGC NNNN NN> N=29+4. Fig. 5, Table 10: <[BDW2009] SQ NN> (Nos 1-17). Fig. 6, Table 11: <[BDW2009] VCC 2062 1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BDW2019]
[BDW2019]	(Becerra+Dichiara+Watson+, 2019) (Not yet in Simbad)
Write:	<<[BDW2019] AN>>
N:	7
Object:	Poss. G (SIMBAD class: Galaxy_Candidate = Galaxy Candidate)
Note:	San Pedro Martir Observatory 1.5m telescope RATIR photometry of N=7 galaxy candidates, in search for GRB 180418A host galaxy. Use of SDSS DR12 data.
Ref:	=2019ApJ...881...12B
by	BECERRA R.L. , DICHIARA S., WATSON A.M., TROJA E., FRAIJA N., KLOTZ A., BUTLER N.R., LEE W.H., VERES P., TURPIN D., BLOOM J.S., BOER M., GONZALEZ J.J., KUTYREV A.S., PROCHASKA J.X., RAMIREZ-RUIZ E., RICHER M.G.
	Astrophys. J., 881, 12-12 (2019)
	Reverse shock emission revealed in early photometry in the candidate short GRB 180418A.
o	Fig. 7, Table 7: <[BDW2019] AN> (Nos G1-G6, S1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Be
Be	(Bernes)
*****	Avoid the usage of Be, prefer [B77]
Details on Acronym: BE
BE	(Bohannan+Epps)
*****	Avoid the usage of BE, prefer [BE74]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Be
Be	(Bernhard+)
*****	Avoid the usage of Be, prefer Brh
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Be
Be	(Berkeley univ.)
*****	Avoid the usage of Be, prefer Berkeley
Details on Acronym: Be
Be	(Be *)
*****	Avoid the usage of Be, prefer [GC2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BE-STIS
BE-STIS	(Bianchi+Efremova, STIS)
Write:	<<BE-STIS NN>>
N:	47
Object:	* (SIMBAD class: Star)
Note:	HST STIS imaging of the galaxy NGC 6822. See also BE-WFPC2.
in source:	NGC 6822
Ref:	=2006AJ....132..378B
by	BIANCHI L. , EFREMOVA B.V.
	Astron. J., 132, 378-392 (2006)
	The recent star formation in NGC 6822 from Hubble Space Telescope imaging.
o	Table 4: <BE-STIS NN> (Nos 1-47). Table 3: <BE-WFPC2 NN> (Nos 1-80).
=E=	Catalogue in electronic form as J/AJ/132/378
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BE-WFPC2
BE-WFPC2	(Bianchi+Efremova, WFPC2)
Write:	<<BE-STIS NN>>
N:	80
Object:	* (SIMBAD class: Star)
Note:	HST WFPC2 imaging of the galaxy NGC 6822. See also BE-STIS.
in source:	NGC 6822
Ref:	=2006AJ....132..378B
by	BIANCHI L. , EFREMOVA B.V.
	Astron. J., 132, 378-392 (2006)
	The recent star formation in NGC 6822 from Hubble Space Telescope imaging.
o	Table 4: <BE-STIS NN> (Nos 1-47). Table 3: <BE-WFPC2 NN> (Nos 1-80).
=E=	Catalogue in electronic form as J/AJ/132/378
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BE74]
[BE74]	(Bohannan+Epps, 1974)= (BE)
Write:	<<[BE74] NNN>>
N:	625
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Note:	Identif. charts
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1974A&AS...18...47B
by	BOHANNAN B. , EPPS H.W.
	Astron. Astrophys., Suppl. Ser., 18, 47-79 (1974)
	H α emission-line stars in the Large Magellanic Cloud. I. A new deep survey.
o	Table 2: <[BE74] NNN> (Nos 1-625)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BE83]
[BE83]	(Braz+Epchtein, 1983)
Write:	<<[BE83] Maser LLL.ll+BB.bbA>> <<[BE83] IR LLL.ll+BB.bbA>>
N:	288+76
Object:	Maser + (IR) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=288 H2O and OH masers, and N=76 sources IR
Ref:	=1983A&AS...54..167B
by	BRAZ M.A. , EPCHTEIN N.
	Astron. Astrophys., Suppl. Ser., 54, 167-185 (1983)
	Catalogue of non stellar molecular maser sources and their probable infrared counterparts in the galactic plane.
o	Tables 1, 1b: <[BE83] Maser LLL.ll+BB.bbA> N=288. Tables 2, 2b: <[BE83] IR LLL.ll+BB.bbA> N=76
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BE99]
[BE99]	(Battinelli+Efremov, 1999)
Write:	<<[BE99] OpCl Clump NN>> <<[BE99] Cepheid Clump NN>> <<[BE99] OpCl-Cepheid Clump N>>
N:	14+17+4
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	Table 1: Clumps of clusters, (Nos 1-14). Table 2: Clumps of cepheids, (Nos 1-17). Table 3: Clumps of clusters within cepheid age-range, (Nos 1-4).
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1999A&A...346..778B
by	BATTINELLI P. , EFREMOV Y.N.
	Astron. Astrophys., 346, 778-784 (1999)
	A comparative study of the spatial distributions of Cepheids and star clusters in the Large Magellanic Cloud.
o	Table 1: <[BE99] OpCl Clump NN> (Nos 1-14). Table 2: <[BE99] Cepheid Clump NN> (Nos 1-17). Table 3: <[BE99] OpCl-Cepheid Clump N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BEA2001]
[BEA2001]	(Beltran+Estalella+Anglada+, 2001)= (VLA)
Write:	<<[BEA2001] Mon R2E NN>> <<[BEA2001] S287 N>> <<[BEA2001] LNNNN N>> <<[BEA2001] PV Cep N>> <<[BEA2001] L1251A NN>> <<[BEA2001] CB247 N>>
N:	66
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio continuum sources detected in 8 regions containing HH outflows..
in source:	[AW90] e
in source:	SH 2-287
in source:	LDN 1654
in source:	LDN 483
in source:	LDN 1203
in source:	LDN 1251A
in source:	[CB88] 247
Ref:	=2001AJ....121.1556B
by	BELTRAN M.T. , ESTALELLA R., ANGLADA G., RODRIGUEZ L.F., TORRELLES J.M.
	Astron. J., 121, 1556-1568 (2001)
	Radio spectral indices of the powering sources of outflows.
o	Table 2: <[BEA2001] Mon R2E NN> (Nos 1-13), <[BEA2001] S287 N> (Nos 1-9), <[BEA2001] L1654 N> (Nos 1-8), <[BEA2001] L483 N> (Nos 1-6), <[BEA2001] L1203 N> (Nos 1-5), <[BEA2001] PV Cep N> (Nos 1-7), <[BEA2001] L1251A N> (Nos 1-9), <[BEA2001] CB247 N> (Nos 1-7).
Ref:	=2004AJ....127.1736R
by	REIPURTH B. , RODRIGUEZ L.F., ANGLADA G., BALLY J.
	Astron. J., 127, 1736-1746 (2004)
	Radio continuum jets from protostellar objects.
o	Table 2: <[RRA2004] Haro 6-10 VLA NA> (Nos 1-3, 1B), <[RRA2004] NGC 2023 MM VLA N> (Nos 1-3), <[RRA2004] NGC 2264 MM VLA N> (Nos 1-8), <[RRA2004] HH 108 VLA N> (Nos 1-2). Text: <[RRA2004] JHHMMSSs+DDMMSS> N=1. Table 2: <[RRC99] VLA NN> (Nos 15-18) added. Table 2: <[RR96] HH 199 N> (Nos 3-4) added. Table 2: <[BEA2001] L1251A NN> (Nos 10-11) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BEB76]
[BEB76]	(Beckwith+Evans+Becklin+, 1976)= (IRS)
Write:	<<[BEB76] IRS Na>> <<[BEB76] IRS NWW>>
N:	8+1+3+6
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	1st ref.: (Nos 1-7), maps in Fig.2 2nd ref.: No. 1a added 3rd ref.: (Nos 3N, 3NE, 3S) added 4th ref.: (Nos 1NE, 1SW, 4N, 4S, 5N, 5S, 9) added IRS 8 is missing
in source:	NAME Mon R2 GMC
Ref:	=1976ApJ...208..390B
by	BECKWITH S. , EVANS II N.J., BECKLIN E.E., NEUGEBAUER G.
	Astrophys. J., 208, 390-395 (1976)
	Infrared observations of Monoceros R2.
o	<[BEB76] IRS N> (Nos 1-7)
Ref:	=1990A&A...235..387A
by	ASPIN C. , WALTHER D.M.
	Astron. Astrophys., 235, 387-394 (1990)
	Infrared imaging polarimetry of Monoceros R2 IRS.
o	Table 1: <[BEB76] IRS 1a>. Table 1: <[AW90] aii> (Nos ai, aii, b-h)
Ref:	=1993AJ....105.1481K
by	KORESKO C.D. , BECKWITH S., GHEZ A.M., MATTHEWS K., HERBST T.M., SMITH D.A.
	Astron. J., 105, 1481-1486 (1993)
	Infrared imges of Monoceros R2 IRS 3: evidence for a circumstellar disk.
o	<[BEB76] IRS NWW> (Nos 3N, 3NE, 3S) added
Ref:	=1994ApJ...425..707H
by	HOWARD E.M. , PIPHER J.L., FORREST W.J.
	Astrophys. J., 425, 707-719 (1994)
	A near-infrared study of the Monoceros R2 star formation region.
o	Table 2: <[AW90] aW> (Nos aN, aS, bN, bS, cN, cS, dN, dS) added. Table 2: <[BEB76] IRS NWW> (Nos 1NE, 1SW, 4N, 4S, 5N, 5S, 9) added
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BEBOP
BEBOP	(Binaries Escorted By Orbiting Planets)
Write:	<<BEBOP -NNN>> <<BEBOP -NNNA>> <<BEBOP -NNNa>>
N:	about 50
Object:	Binary * + * + Poss. Pl (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	The BEBOP survey is search for circumbinary planets orbiting main sequence binary stars, using radial velocities. The BEBOP designation will be given to systems detected with radial-velocities.
Notes:	We are about to submit our first detection, BEBOP-1.
Auth.:	Amaury Triaud University of Birmingham
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [BEC2010]
[BEC2010]	(Herschel Reference Sample)= (HRS)
Write:	<<[BEC2010] HRS NNN>>
N:	323
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Sample of N=323 galaxies of the Herschel Reference Survey (a Herschel guaranteed time key project).
Ref:	=2010PASP..122..261B
by	BOSELLI A. , EALES S., CORTESE L., BENDO G., CHANIAL P., BUAT V., DAVIES J., AULD R., RIGBY E., BAES M., BARLOW M., BOCK J., BRADFORD M., CASTRO-RODRIGUEZ N., CHARLOT S., CLEMENTS D., CORMIER D., DWEK E., ELBAZ D., GALAMETZ M., GALLIANO F., GEAR W., GLENN J., GOMEZ H., GRIFFIN M., HONY S., ISAAK K., LEVENSON L., LU N., MADDEN S., O'HALLORAN B., OKAMURA K., OLIVER S., PAGE M., PANUZZO P., PAPAGEORGIOU A., PARKIN T., PEREZ-FOURNON I., POHLEN M., RANGWALA N., ROUSSEL H., RYKALA A., SACCHI N., SAUVAGE M., SCHULZ B., SCHIRM M., SMITH M.W.L., SPINOGLIO L., STEVENS J., SYMEONIDIS M., VACCARI M., VIGROUX L., WILSON C., WOZNIAK H., WRIGHT G., ZEILINGER W.
	PASP, 122, 261-287 (2010)
	The Herschel Reference Survey.
o	Table 1: <[BEC2010] HRS NNN> (Nos 1-323).
=E=	Catalogue in electronic form as J/PASP/122/261
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BEE
BEE	(Bower+Ellis+Efstathiou)
Write:	<<BEE NN>> <<BEE ggg>>
N:	31+2
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	N=31 G among (Nos 1-68), and N=2 G format ggg for greek letters alf and bet Plate of the core.
in source:	ACO 2029
Ref:	=1988MNRAS.234..725B
by	BOWER R.G. , ELLIS R.S., EFSTATHIOU G.
	Mon. Not. R. Astron. Soc., 234, 725-732 (1988)
	A study of satellite galaxies in the rich cluster A 2029.
o	cD galaxy in table 2 = Z 1508.4+0556
o	<BEE NN> N=31 among (Nos 1-68), <BEE alp>, <BEE bet>.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BEF2020]
[BEF2020]	(Brightman+Earnshaw+Furst+, 2020)
Write:	<<[BEF2020] M51 XT-1>>
N:	1
Object:	ULX (SIMBAD class: ULX = Ultra-luminous X-ray Source)
Note:	Swift XRT observations of N=1 ultraluminous X-ray source (ULX) in M51.
in source:	NGC 5194 = M 51
Ref:	=2020ApJ...895..127B
by	BRIGHTMAN M. , EARNSHAW H., FURST F., HARRISON F.A., HEIDA M., ISRAEL G., PIKE S., STERN D., WALTON D.J.
	Astrophys. J., 895, 127-127 (2020)
	Swift monitoring of M51: a 38 day superorbital period for the pulsar ULX7 and a new transient ultraluminous X-ray source.
o	<[BEF2020] M51 XT-1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BEG2008]
[BEG2008]	(Beltran+Estalella+Girart+, 2008)= (OVRO)
Write:	<<[BEG2008] OVRO N>>
N:	3
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	OVRO mm continuum observations toward IRAS 20050+2720.
Ref:	=2008A&A...481...93B
by	BELTRAN M.T. , ESTALELLA R., GIRART J.M., HO P.T.P., ANGLADA G.
	Astron. Astrophys., 481, 93-105 (2008)
	On the nature of outflows in intermediate-mass protostars: a case study of IRAS 20050+2720.
o	Paragraph 2.1 QSO J2015+71 is a misprint for QSO J2015+371.
o	Table 2: <[BEG2008] OVRO N> (Nos 1-3).
=E=	Catalogue in electronic form as <J/A+A/481/93/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BEH2002]
[BEH2002]	(Beltran+Estalella+Ho+, 2002)= (VLA)
Write:	<<[BEH2002] VLA N>>
N:	5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
in source:	LDN 1634
Ref:	=2002ApJ...565.1069B
by	BELTRAN M.T. , ESTALELLA R., HO P.T.P., CALVET N., ANGLADA G., SEPULVEDA I.
	Astrophys. J., 565, 1069-1083 (2002)
	Multiwavelength study of the powering sources of the double H_{2} bipolar jet in L1634.
o	IRS 7 = [HL95] LDN 1634 7
o	Fig.2, Table 3: <[BEH2002] VLA N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BEH2009]
[BEH2009]	(Belokurov+Evans+Hewett+, 2009)
Write:	<<[BEH2009] CSWA 2 LN>> <<[BEH2009] CSWA 3 L>> <<[BEH2009] CSWA N A>>
Object:	Grav. lens + Grav. lensed image of a G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	SAO 6m, Calar Alto 3.5m, INT 2.5m and WHT 4.2m follow-up observations of N=2 gravitational lenses from the CASSOWARY survey. See also CSWA.
in source:	CSWA 2
in source:	CSWA 3
Ref:	=2009MNRAS.392..104B
by	BELOKUROV V. , EVANS N.W., HEWETT P.C., MOISEEV A., McMAHON R.G., SANCHEZ S.F., KING L.J.
	Mon. Not. R. Astron. Soc., 392, 104-112 (2009)
	Two new large-separation gravitational lenses from SDSS.
o	Fig. 1, Tables 1-2: <CSWA NN> N=7 among (Nos 1-13). Fig.4, Table 2: <[BEH2009] CSWA 2 LN> (Nos L1-L2), <[BEH2009] CSWA 2 A> (Nos A-G). Fig. 4, Table 3: <[BEH2009] CSWA 3 L>, <[BEH2009] CSWA 3 A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BEH2012]
[BEH2012]	(Bianchi+Efremova+Hodge+, 2012)
Write:	<<[BEH2012] Phoenix NNNN>> <<[BEH2012] Pegasus NNNN>> <<[BEH2012] Sextans A NNNN>> <<[BEH2012] Sextans B NNNN>> <<[BEH2012] WLM NNNN>> <<[BEH2012] NGC 6822 NNNNN>> <<[BEH2012] M31 NNNNNN>>
N:	1486+2204+4148+3583+7058+26722
Object:	* (SIMBAD class: Star)
Note:	HST WPFC2 multi-band photometry of galaxies in the Local Group.
in source:	NAME Phe Dwarf Irregular
in source:	NAME Pegasus Galaxy
in source:	NAME Sextans A
in source:	NAME Sextans B
in source:	DDO 221 = WLM Galaxy
in source:	NGC 6822
in source:	M 31 = NGC 224
Ref:	=2012AJ....143...74B
by	BIANCHI L. , EFREMOVA B., HODGE P., MASSEY P., OLSEN K.A.G.
	Astron. J., 143, 74 (2012)
	A treasury study of star-forming regions in the Local Group. I. HST photometry of young populations in six dwarf galaxies.
o	Table 4: <[BEH2012] Phoenix NNNN> (Nos 0-1485), <[BEH2012] Pegasus NNNN> (Nos 0-2203), <[BEH2012] Sextans A NNNN> (Nos 0-4148), <[BEH2012] Sextans B NNNN> (Nos 0-3583), <[BEH2012] WLM NNNN> (Nos 0-7057), <[BEH2012] NGC 6822 NNNNN> (Nos 0-26721).
Ref:	=2012AJ....144..142B
by	BIANCHI L. , EFREMOVA B., HODGE P., KANG Y.
	Astron. J., 144, 142 (2012)
	A Hubble Space Telescope treasury study of star-forming regions in the Local Group. II. Young stellar populations in M31.
o	Table 2: <[BEH2012] M31 NNNNNN> (Nos 0-118035).
o	OB10-64 is MAC 3-64 in Simbad.
=E=	Catalogue in electronic form as <J/AJ/143/74/>
=E=	Catalogue in electronic form as <J/AJ/144/142/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BEJ2007]
[BEJ2007]	(Breen+Ellingsen+Johnston-Hollitt+, 2007) (Not yet in Simbad)
Write:	<<[BEJ2007] N>>
N:	9
Object:	H2O Maser (SIMBAD class: Maser)
Note:	ATCA observations to search for H2O masers associated with RCW 106.
Ref:	=2007MNRAS.377..491B
by	BREEN S.L. , ELLINGSEN S.P., JOHNSTON-HOLLITT M., WOTHERSPOON S., BAINS I., BURTON M.G., CUNNINGHAM M., LO N., SENKBEIL C.E., WONG T.
	Mon. Not. R. Astron. Soc., 377, 491-506 (2007)
	A search for 22-GHz water masers within the giant molecular cloud associated with RCW 106.
o	Table 1: <[BEJ2007] N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BEK2006]
[BEK2006]	(Bastian+Emsellem+Kissler-Patig+, 2006)
Write:	<<[BEK2006] Complex Na>> <<[BEK2006] Nuc N>>
N:	6+2+2
Object:	Star Cluster Complex (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	Integral field spectroscopy of young star complexes detected in The Antennae from HST archival data. VIMOS-VLT observations. N=6 complexes in the overlap region in NGC 4038, and N=2 in the nuclear region of NGC 4038. See also [WZL99], [WGL2005]
in source:	NAME the Antennae
Ref:	=2006A&A...445..471B
by	BASTIAN N. , EMSELLEM E., KISSLER-PATIG M., MARASTON C.
	Astron. Astrophys., 445, 471-483 (2006)
	Young star cluster complexes in NGC 4038/39. Integral field spectroscopy using VIMOS-VLT.
o	Table 1, Fig.2: <[BEK2006] Complex Na> (Nos 1-6, 3a-3b). Table 1, Fig.3: <[BEK2006] Nuc N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BEL81]
[BEL81]	(Bergvall+Ekman+Lauberts, 1981) (Not yet in Simbad)
Write:	<<[BEL81] a>> <<[BEL81] aN>>
N:	6+6
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Note:	ESO 255-7 is a small group of 3 galaxies (Nos a-c), with 3 other objects very faint, stars or companions (Nos d-f).
in source:	ESO 255-7
Ref:	=1981A&A....95..266B
by	BERGVALL N. , EKMAN A., LAUBERTS A.
	Astron. Astrophys., 95, 266-277 (1981)
	ESO 255-IG 07, a compact group of interacting galaxies.
o	Tables 1, 2, Fig.4: <[BEL81] a> (Nos a-f), <[BEL81] aN> (Nos a0, a1, b0, b1, c1, c2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BEM
BEM	(Bohannan EM. obj.)
*****	Avoid the usage of BEM, prefer [BCM85]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [BEM2002]
[BEM2002]	(Bagchi+Ensslin+Miniati+, 2002)
Write:	<<[BEM2002] GN>>
N:	4
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
in source:	ZwCl 2341+0000
Ref:	=2002NewA....7..249B
by	BAGCHI J. , ENSSLIN T.A., MINIATI F., STALIN C.S., SINGH M., RAYCHAUDHURY S., HUMESHKAR N.B.
	New Astronomy, 7, 249-277 (2002)
	Evidence for shock acceleration and intergalactic magnetic fields in a large-scale filament of galaxies ZwCl 2341.1+0000.
o	Table 1, Fig.1: <[BEM2002] GN> (Nos G1-G4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BEM91]
[BEM91]	(Bothun+Elias+McAlpine, 1991)= (C*)
Write:	<<[BEM91] NN>>
N:	31
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Note:	The authors use a format 'CNN' for Carbon (Nos 1-32) No. 6 missing also 'HNN' (Helium ), or 'MNN' (M ) (not in SIMBAD)
Ref:	=1991AJ....101.2220B
by	BOTHUN G. , ELIAS J.H., MacALPINE G., MATTHEWS K., MOULD J.R., NEUGEBAUER G., REID I.N.
	Astron. J., 101, 2220-None (1991)
	Carbon stars at high galactic latitude.
o	<[BEM91] NN> (Nos 1-32), No. 6 missing
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BEP2016]
[BEP2016]	(Busquet+Estalella+Palau+, 2016)
Write:	<<[BEP2016] Hub-W MMNa>>
N:	9+17
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	SMA 1.3mm continuum observations of N=9+17 submillimeter sources toward the two hubs of the IR dark cloud G014.225-0.506.
in source:	M 17:NAME M17 SWex = NAME M17 SWex
Ref:	=2016ApJ...819..139B
by	BUSQUET G. , ESTALELLA R., PALAU A., LIU H.B., ZHANG Q., GIRART J.M., DE GREGORIO-MONSALVO I., PILLAI T., ANGLADA G., HO P.T.P.
	Astrophys. J., 819, 139 (2016)
	What is controlling the fragmentation in the infrared dark cloud G14.225-0.506?: different levels of fragmentation in twin hubs.
o	Table 4: <[BEP2016] Hub-N MMNa> N=9 (Nos MM1a-MM1g, MM2, MM3), <[BEP2016] Hub-S MMa> N=17 (Nos MM1a to MM9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BeppoSAX
BeppoSAX	(BeppoSAX instrument)= (SAX)
Write:	<<NAME BeppoSAX source a>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Ref:	=1997IAUC.6539Q...1B
by	BUTLER R.C. , PIRO L., COSTA E., FEROCI M., FRONTERA F., DAL FIUME D., HEISE J., JAGER R., SACCO B., CHIAPPETTI L., PARMAR A., ANTONELLI L.A., RICCI D., MULLER J.M., COLETTA A., DE LIBERO C., SALOTTI L., VOGES W., BOLLER T., GREINER J.
	IAU Circ., 6539, 1-None (1997)
	GRB 970111.
o	<[BPC97] source a> (Nos a-b), <[BPC97] source N> (Nos 1-3).
Origin	of the Acronym: A (1997IAUC.6545Q...1F,1997IAUC.6567R...1F)
Details on Acronym: Ber
Ber	(Bernes)
*****	Avoid the usage of Ber, prefer [B77]
Details on Acronym: Berkeley
Berkeley	(Berkeley univ.)= (Be)
Write:	<<Cl Berkeley NNN>>
N:	104?
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Note:	Lynga 1979, see C, gives 90 clusters numbered between 1 and 104. First published in the first edition of the Catalogue of Star Clusters and Associations, 1958.
Details on Acronym: Bernacca
Bernacca	(Bernacca) (Not yet in Simbad)
Write:	<<Bernacca Ra NNNN>>
N:	3075
Object:	* (SIMBAD class: Star)
Note:	In the format 'R' stands for: I : Main sequence single stars (Nos 1-1005). II : Main sequence spectroscopic binaries and eclipsing systems (Nos 1-360). IIIa : Be and shell stars (Nos 1-189). IIIb : Bp, Ap, Apec and Am stars (Nos 1-243). IV : Evolved stars (Nos 1-1278).
Ref:	=1970CoAsi.239....1B
by	BERNACCA P.L. , PERINOTTO M.
	Contr. Oss. Astrof. Padova in Asiago, 239, 1-None (1970)
	A catalogue of stellar rotational velocities.
o	Catalogue I: <Bernacca I NNNN> (Nos 1-1005). Catalogue II: <Bernacca II NNN> (Nos 1-360)
Ref:	=1971CoAsi.250....1B
by	BERNACCA P.L. , PERINOTTO M.
	Contr. Oss. Astrof. Padova in Asiago, 250, 1-None (1971)
	A catalogue of stellar rotational velocities. III. Stars with peculiar spectrum.
o	Catalogue III: <Bernacca IIIa NNN> (Nos 1-189), <Bernacca IIIb NNN> (Nos 1-243).
Ref:	=1973CoAsi.294....1B
by	BERNACCA P.L.
	Contr. Oss. Astrof. Padova in Asiago, 294, 1-None (1973)
	A catalogue of stellar rotational velocities. IV. Evolved stars.
o	Catalogue IV: <Bernacca IV NNNN> (Nos 1-1278)
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: Bernes
Bernes	(Bernes)
*****	Avoid the usage of Bernes, prefer [B77]
Details on Acronym: BES
BES	(Broadhurst+Ellis+Shanks)
Write:	<<BES FFF NN>> <<BES AAA NN>>
N:	236
Object:	Faint G (SIMBAD class: Galaxy)
Note:	AAT FOCAP spectroscopy of galaxies in five fields.
Ref:	=1988MNRAS.235..827B
by	BROADHURST T.J. , ELLIS R.S., SHANKS T.
	Mon. Not. R. Astron. Soc., 235, 827-856 (1988)
	The Durham/Anglo-Australian telescope faint galaxy redshift survey.
o	Table 3: <BES SGP NNN> (Nos 1-71), <BES 197 NN> (Nos 1-39), <BES MT NN> (Nos 1-44), <BES 419 NN> (Nos 1-38), <BES 529 NN> (Nos 1-44)
=E=	Catalogue in electronic form as J/MNRAS/235/827
Details on Acronym: [BES2005]
[BES2005]	(Bradac+Erben+Schneider+ 2005)
Write:	<<[BES2005] A>> <<[BES2005] AN>> <<[BES2005] AC>>
N:	13+1
Object:	Arc (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Stat:	is completely incorporated in Simbad
Note:	VLT ESO observations of the RX J1347.5-1145 cluster of G. New arc candidates. 'AC' is a possible counterimage to A4 and A5. See also [SSK98], [SGE95].
in source:	ClG J1347-1145 = RX J1347.5-1145
Ref:	=2005A&A...437...49B
by	BRADAC M. , ERBEN T., SCHNEIDER P., HILDEBRANDT H., LOMBARDI M., SCHIRMER M., MIRALLES J.-M., CLOWE D., SCHINDLER S.
	Astron. Astrophys., 437, 49-60 (2005)
	Strong and weak lensing united. II. The cluster mass distribution of the most X-ray luminous cluster RX J1347.5-1145.
o	Table 2: <[BES2005] AN> (Nos A1-A5, B1-B2, C, D1-D4, E), <[BES2005] AC> (No.AC).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BEST
BEST	(Berlin Exoplanet Search Telescope)
*****	Avoid the usage of BEST, prefer [FKC2012]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BEST
BEST	(Berlin Exoplanet Search Telescope)
*****	Avoid the usage of BEST, prefer [KCP2016]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BEST
BEST	(Berlin Exoplanet Search Telescope)
*****	Avoid the usage of BEST, prefer [KEE2007]
Origin	of the Acronym: A = Assigned by the author(s)
History	of this Acronym: replaced by [KEE2007]
Details on Acronym: BEST
BEST	(Berlin Exoplanet Search Telescope)
*****	Avoid the usage of BEST, prefer [KEE2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BEST
BEST	(Berlin Exoplanet Search Telescope)
*****	Avoid the usage of BEST, prefer [PCC2011c]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BEST II
BEST II	(Berlin Exoplanet Search Telescope II) (Not yet in Simbad)
*****	Avoid the usage of BEST II, prefer [DCT2018]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BEST II
BEST II	(Berlin Exoplanet Search Telescope II)
*****	Avoid the usage of BEST II, prefer [FCC2013]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BEV78]
[BEV78]	(Blair+Evans+Vanden Bout+, 1978) (Not yet in Simbad)
Write:	<<[BEV78] S140 IR>> <<[BEV78] S140 N>> <<[BEV78] Shell N>>
N:	1+6+6
Object:	(IR) + Cloud (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 3: N=1 strong (IR) source, name 'S140 IR', + N=6 (IR) sources, (Nos 1-6) in Sh 2-140 Table 6: N=6 Shells in Sh 2-140
in source:	SH 2-140
Ref:	=1978ApJ...219..896B
by	BLAIR G.N. , EVANS II N.J., VANDEN BOUT P.A., PETERS III W.L.
	Astrophys. J., 219, 896-913 (1978)
	The energetics of molecular clouds. II. The S140 molecular cloud.
o	Table 3: <[BEV78] S140 IR> = <NAME SH 2-140 IR>, <[BEV78] S140 N> (Nos 1-6). Table 6: <[BEV78] Shell N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BEV98]
[BEV98]	(Bade+Engels+Voges+, 1998)
Write:	<<[BEV98] RX JHHMM.m+DDMM NNN>>
N:	10528
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Hamburg-RASS catalogue of possible optical identifications.
Ref:	=1998A&AS..127..145B
by	BADE N. , ENGELS D., VOGES W., BECKMANN V., BOLLER T., CORDIS L., DAHLEM M., ENGLHAUSER J., MOLTHAGEN K., NASS P., STUDT J., REIMERS D.
	Astron. Astrophys., Suppl. Ser., 127, 145-152 (1998)
	The Hamburg/RASS Catalogue of optical identifications.
o	optical catalogues: <[BEV98] RX JHHMM.m+DDMM NNN> N=10528.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BEZ2011]
[BEZ2011]	(Busquet+Estalella+Zhang+, 2011)
Write:	<<[BEZ2011] AA>> <<[BEZ2011] J053048.01+334754.1>>
N:	3+1
Object:	Core (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	CARMA observations of N=3 cores and N=1 3.2mm source in the protostellar cluster RAFGL 5142.
in source:	RAFGL 5142
Ref:	=2011A&A...525A.141B
by	BUSQUET G. , ESTALELLA R., ZHANG Q., VITI S., PALAU A., HO P.T.P., SANCHEZ-MONGE A.
	Astron. Astrophys., 525A, 141-141 (2011)
	N_{2}H^+ depletion in the massive protostellar cluster AFGL 5142.
o	Fig. 4, Table 1: <[BEZ2011] AA> (Nos CC, EC, WC). Paragr. 3.1: <[BEZ2011] J053048.01+334754.1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BF
BF	(Barbier-Brossat+Figon)
*****	Avoid the usage of BF, prefer [BF2000]
Origin	of the Acronym: L (2001A&A...380..435S)
Details on Acronym: BF
BF	(Bologna obs., Faint?)
*****	Avoid the usage of BF, prefer BVF
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BF2000]
[BF2000]	(Barbier-Brossat+Figon, 2000)= (BF)
Write:	<<[BF2000] NNNNN>>
N:	36145
Object:	* (SIMBAD class: Star)
Ref:	=2000A&AS..142..217B
by	BARBIER-BROSSAT M. , FIGON P.
	Astron. Astrophys., Suppl. Ser., 142, 217-223 (2000)
	Catalogue general de vitesses radiales moyennes pour les etoiles galactiques. Mean radial velocities catalog of galactic stars.
o	Catalogue: <[BF2000] NNNNN> (Nos 1-36145).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BF64]
[BF64]	(Blanco+Fitzgerald, 1964)= (BlFg) (Not yet in Simbad)
Write:	<<[BF64] NN>>
N:	26
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Ref:	=1964PASP...76..438B
by	BLANCO V.M. , FITZGERALD M.P.
	Publ. Astron. Soc. Pac., 76, 438-439 (1964)
	Faint H-α emission objects near ζ Cephei.
o	Table I: <[BF64] NN> (Nos 1-26)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BF76
BF76	(Becker+Fenkart, 1976)
*****	Avoid the usage of BF76, prefer Basel
Origin	of the Acronym: L (1997BaltA...6..499B)
Details on Acronym: [BF76]
[BF76]	(Bridle+Fomalont, 1976)
Write:	<<[BF76] A>> <<[BF76] A(aaa)>> <<[BF76] N>>
N:	8+13+5
Object:	(Rad) + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=8 galaxies in ACO 2256 (Nos 1-8). Radio features in ACO 2256, (Nos A-M), Nos C and F have components (Nos C(i), C(ii), F(i), F(ii), F(iii)). (Nos A-M) are identical to [RSM94] A to M. See also [RSM94]. Table 1: N=8 galaxies in ACO 2256.
in source:	ACO 2256
Ref:	=1976A&A....52..107B
by	BRIDLE A.H. , FOMALONT E.B.
	Astron. Astrophys., 52, 107-113 (1976)
	Complex radio emission from the X-ray cluster Abell 2256.
o	Fig.2: <[BF76] A> (Nos A-H). Table 1: <[BF76] N> (Nos 1-8).
Ref:	=1979A&A....80..201B
by	BRIDLE A.H. , FOMALONT E.B., MILEY G.K., VALENTIJN E.A.
	Astron. Astrophys., 80, 201-211 (1979)
	The radio properties of the X-ray cluster Abell 2256.
o	Fig.1, Table 2: <[BF76] A> (Nos I-M) added, <[BF76] A(aaa)> (Nos C(i), C(ii), F(i), F(ii), F(iii)).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFA97]
[BFA97]	(Brosch+Formiggini+Almoznino+, 1997)= (FAUST)
Write:	<<[BFA97] NNN>>
N:	191
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	Observations of the FAUST telescope on ATLAS 1. See also [BOA98]
in source:	NAME Virgo Cluster
Ref:	=1997ApJS..111..143B
by	BROSCH N. , FORMIGGINI L., ALMOZNINO E., SASSEEN T., LAMPTON M., BOWYER S.
	Astrophys. J., Suppl. Ser., 111, 143-161 (1997)
	FAUST observations of ultraviolet sources toward the Virgo cluster.
o	Table 1: <[BFA97] NNN> (Nos 1-191)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFB2004]
[BFB2004]	(Benitez+Ford+Bouwens+, 2004)= ([BFB2004a])
Write:	<<[BFB2004] VV 29 NNNN>> <<[BFB2004] NGC 4676 NNNN>>
N:	5712+3254
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Analysis of faint galaxy population in the HST Advanced Camera for Surveys (ACS) Early Release fields VV 29 and NGC 4676.
Ref:	=2004ApJS..150....1B
by	BENITEZ N. , FORD H., BOUWENS R., MENANTEAU F., BLAKESLEE J., GRONWALL C., ILLINGWORTH G., MEURER G., BROADHURST T.J., CLAMPIN M., FRANX M., HARTIG G.F., MAGEE D., SIRIANNI M., ARDILA D.R., BARTKO F., BROWN R.A., BURROWS C.J., CHENG E.S., CROSS N.J.G., FELDMAN P.D., GOLIMOWSKI D.A., INFANTE L., KIMBLE R.A., KRIST J.E., LESSER M.P., LEVAY Z., MARTEL A.R., MILEY G.K., POSTMAN M., ROSATI P., SPARKS W.B., TRAN H.D., TSVETANOV Z.I., WHITE R.L., ZHENG W.
	Astrophys. J., Suppl. Ser., 150, 1-None (2004)
	Faint galaxies in deep advanced camera for surveys observations.
o	Table 4: <[BFB2004] VV 29 NNNN> (Nos 1-5712). Table 5: <[BFB2004] NGC 4676 NNNN> (Nos 1-3254).
=E=	Catalogue in electronic form as J/ApJS/150/1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFB2004a]
[BFB2004a]	(Benitez+Ford+Bouwens+, 2004)
*****	Avoid the usage of [BFB2004a], prefer [BFB2004]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFB2004b]
[BFB2004b]	(Beasley+Forbes+Brodie+, 2004)
Write:	<<[BFB2004b] KNNN>>
N:	41
Object:	GlCl + G + * (SIMBAD class: GlobCluster = Globular Cluster)
Note:	Keck Low-Resolution Imaging Spectrometer is used to search for globular clusters in NGC 524. Among the 41 objects observed, 29 are globular clusters, 9 are galaxies and 3 are stars.
in source:	NGC 524
Ref:	=2004MNRAS.347.1150B
by	BEASLEY M.A. , FORBES D.A., BRODIE J.P., KISSLER-PATIG M.
	Mon. Not. R. Astron. Soc., 347, 1150-1163 (2004)
	Keck spectroscopy and imaging of globular clusters in the lenticular galaxy NGC 524.
o	Table 1: <[BFB2004b] KNNN> N=41 among (Nos K004-K115).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFB2007]
[BFB2007]	(Braine+Ferguson+Bertoldi+, 2007)
Write:	<<[BFB2007] NGC 6946 PNN>>
N:	10
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	IRAM 30m telescope CO(1-0) and CO(2-1) line observations of N=10 molecular clouds in the far outskirts of NGC 6946.
Ref:	=2007ApJ...669L..73B
by	BRAINE J. , FERGUSON A.M.N., BERTOLDI F., WILSON C.D.
	Astrophys. J., 669L, 73-76 (2007)
	The detection of molecular gas in the outskirts of NGC 6946.
o	Table 1: <[BFB2007] NGC 6946 PNN> (N=10 among Nos P2-P12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFB2010]
[BFB2010]	(Bian+Fan+Bechtold+, 2010) (Not yet in Simbad)
Write:	<<[BFB2010] AN>>
N:	3
Object:	Grav. lensed image + Grav. lens (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	LBT LUCIFER1 (NIR) observations of N=1 gravitational arc and N=2 lens galaxies in the gravitational lens system [DAA2009] SDSS J090002.79+223403.6.
in source:	[DAA2009] SDSS J090002.79+223403.6
Ref:	=2010ApJ...725.1877B
by	BIAN F. , FAN X., BECHTOLD J., McGREER I.D., JUST D.W., SAND D.J., GREEN R.F., THOMPSON D., PENG C.Y., SEIFERT W., AGEORGES N., JUETTE M., KNIERIM V., BUSCHKAMP P.
	Astrophys. J., 725, 1877-1885 (2010)
	LBT/LUCIFER observations of the z ~ 2 lensed galaxy J0900+2234.
o	Figs 1-2, Table 2: <[BFB2010] AN> (Nos A1, G1-G2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFB2012]
[BFB2012]	(Bernard+Ferguson+Barker+, 2012)
Write:	<<[BFB2012] VNN>>
N:	25
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations of N=12+13 RR Lyr stars respectively in the warp in the stellar disc and in the outer disc of M31.
in source:	M 31 = NGC 224
Ref:	=2012MNRAS.420.2625B
by	BERNARD E.J. , FERGUSON A.M.N., BARKER M.K., HIDALGO S.L., IBATA R.A., IRWIN M.J., LEWIS G.F., McCONNACHIE A.W., MONELLI M., CHAPMAN S.C.
	Mon. Not. R. Astron. Soc., 420, 2625-2643 (2012)
	The star formation history and dust content in the far outer disc of M31.
o	Tables 2-3: <[BFB2012] VNN> (Nos V01-V25).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BFC
BFC	(Batten+Fletcher+McCarthy)
*****	Avoid the usage of BFC, prefer SBC8
Origin	of the Acronym: L (1996A&A...313..523B)
Details on Acronym: [BFC2018]
[BFC2018]	(Boselli+Fossati+Consolandi+, 2018) (Not yet in Simbad)
Write:	<<[BFC2018] NGC 4424 PS1>>
N:	1
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	N=1 X-ray source to the south-east of the nucleaus of NGC 4424. Use of Chandra and XMM-Newton data.
in source:	NGC 4424
Ref:	=2018A&A...620A.164B
by	BOSELLI A. , FOSSATI M., CONSOLANDI G., AMRAM P., GE C., SUN M., ANDERSON J.P., BOISSIER S., BOQUIEN M., BUAT V., BURGARELLA D., CORTESE L., COTE P., CUILLANDRE J.C., DURRELL P., EPINAT B., FERRARESE L., FUMAGALLI M., GALBANY L., GAVAZZI G., GOMEZ-LOPEZ J.A., GWYN S., HENSLER G., KUNCARAYAKTI H., MARCELIN M., MENDES DE OLIVEIRA C., QUINT B.C., ROEDIGER J., ROEHLLY Y., SANCHEZ S.F., SANCHEZ-JANSSEN R., TOLOBA E., TRINCHIERI G., VOLLMER B.
	Astron. Astrophys., 620A, 164-164 (2018)
	A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE). IV. A tail of ionised gas in the merger remnant NGC4424.
o	Fig. 5: <[BFC2018] NGC 4424 PS1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFC81]
[BFC81]	(Bridle+Fomalont+Cornwell, 1981)
Write:	<<[BFC81] 3C 293 A>> <<[BFC81] 3C 293 Radio Core>> <<[BFC81] 3C 293 Opt Knot>> <<[BFC81] 3C 293 West>> <<[BFC81] 3C 293 East>> <<[BFC81] 3C 293 Mid>> <<[BFC81] 3C 293 WN>>
N:	4+1+1+3+5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA, MERLIN, GMRT, and VLBI observations of the structure of 3C 293.
in source:	3C 293
Ref:	=1981AJ.....86.1294B
by	BRIDLE A.H. , FOMALONT E.B., CORNWELL T.J.
	Astron. J., 86, 1294-1305 (1981)
	The large and small-scale structure of 3C 293.
o	Table II: <[BFC81] 3C 293 A> (Nos A-D), <[BFC81] 3C 293 Radio Core> N=1, <[BFC81] 3C 293 Opt Knot> N=1.
Ref:	=2002MNRAS.329..620B
by	BESWICK R.J. , PEDLAR A., HOLLOWAY A.J.
	Mon. Not. R. Astron. Soc., 329, 620-628 (2002)
	A radio study of neutral gas and dust in the radio galaxy 3C 293.
o	Table 1: <[BFC81] 3C 293 West>, <[BFC81] 3C 293 East>, <[BFC81] 3C 293 Mid>, N=3 added.
Ref:	=2004MNRAS.352...49B
by	BESWICK R.J. , PECK A.B., TAYLOR G.B., GIOVANNINI G.
	Mon. Not. R. Astron. Soc., 352, 49-60 (2004)
	High-resolution imaging of the radio continuum and neutral gas in the inner kiloparsec of the radio galaxy 3C 293.
o	HI absorption line properties measurement regions (Table 3) not in SIMBAD.
o	Fig.3, Table 2: <[BFC81] 3C 293 WN> (Nos E1-E3, W1-W2) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFE95]
[BFE95]	(Bade+Fink+Engels+, 1995)
Write:	<<[BFE95] NNNa>>
N:	284
Object:	QSO (SIMBAD class: AGN = Active Galaxy Nucleus)
Note:	ROSAT All-Sky Survey
Ref:	=1995A&AS..110..469B
by	BADE N. , FINK H.H., ENGELS D., VOGES W., HAGEN H.-J., WISOTZKI L., REIMERS D.
	Astron. Astrophys., Suppl. Ser., 110, 469-511 (1995)
	AGN from the ROSAT all-sky survey.
o	Table 3: <[BFE95] NNNa> (Nos 1-49, 50a, 50b, 51-283)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFF2014]
[BFF2014]	(Blom+Forbes+Foster+, 2014)
Write:	<<[BFF2014] NN>>
N:	31
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Note:	Keck II DEIMOS observations of N=31 globular clusters in NGC 4342 and the stellar stream. Use of archival CFHT MegaCam data.
in source:	NGC 4342
Ref:	=2014MNRAS.439.2420B
by	BLOM C. , FORBES D.A., FOSTER C., ROMANOWSKY A.J., BRODIE J.P.
	Mon. Not. R. Astron. Soc., 439, 2420-2431 (2014)
	The SLUGGS Survey: new evidence for a tidal interaction between the early-type galaxies NGC 4365 and NGC 4342.
o	Table 1: <[BFF2014] NN> (Nos 1-31).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFG2000]
[BFG2000]	(Brogan+Frail+Goss+, 2000) (Not yet in Simbad)
Write:	<<[BFG2000] W51C N>> <<[BFG2000] GLLL.l+b.B N>> <<[BFG2000] CTB 37A N>> <<[BFG2000] CTB 33 N>>
N:	12
Object:	OH Maser (SIMBAD class: Maser)
Note:	N=12 OH masers in 5 SNR
in source:	W 51:W 51C = W 51C
in source:	SNR G349.7+00.2
in source:	CTB 37
in source:	CTB 33
in source:	SNR G357.7-00.1
Ref:	=2000ApJ...537..875B
by	BROGAN C.L. , FRAIL D.A., GOSS W.M., TROLAND T.H.
	Astrophys. J., 537, 875-890 (2000)
	OH Zeeman magnetic field detections toward five supernova remnants using the VLA.
o	Table 2: <[BFG2000] W51C N> (Nos 1-2), <[BFG2000] G349.7+0.2 N> (Nos 1-3), <[BFG2000] CTB 37A N> (Nos 1-5), <[BFG2000] CTB 33 N> (No. 1), <[BFG2000] G357.7-0.1 N> (No. 1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFG2003]
[BFG2003]	(Bacchi+Feretti+Giovannini+, 2003)
Write:	<<[BFG2003] ANNNN SN>>
N:	2+4+8+9+7+6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA 1.4GHz observations of 6 ACO clusters of galaxies.
in source:	ACO 401
in source:	ACO 545
in source:	ACO 754
in source:	ACO 1914
in source:	ACO 2219
in source:	ACO 2390
Ref:	=2003A&A...400..465B
by	BACCHI M. , FERETTI L., GIOVANNINI G., GOVONI F.
	Astron. Astrophys., 400, 465-476 (2003)
	Deep images of cluster radio halos.
o	Fig.1: <[BFG2003] A401 SN> (Nos S1-S2). Fig.2: <[BFG2003] A545 SN> (Nos S1-S4). Fig.3: <[BFG2003] A754 SN> (Nos S1-S8). Fig.6: <[BFG2003] A1914 SN> (Nos S1-S9). Fig.9: <[BFG2003] A2219 SN> (Nos S1-S7). Fig.10: <[BFG2003] A2390 SN> (Nos S1-S6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFG2009]
[BFG2009]	(Bonafede+Feretti+Giovannini+, 2009)
Write:	<<[BFG2009] A>>
N:	4
Object:	rG (SIMBAD class: RadioG = Radio Galaxy)
Note:	VLA 20 and 6cm observations of MACS J0717.5+3745.
in source:	ClG J0717+3745 = MCS J0717.5+3745
Ref:	=2009A&A...503..707B
by	BONAFEDE A. , FERETTI L., GIOVANNINI G., GOVONI F., MURGIA M., TAYLOR G.B., EBELING H., ALLEN S., GENTILE G., PIHLSTROEM Y.
	Astron. Astrophys., 503, 707-720 (2009)
	Revealing the magnetic field in a distant galaxy cluster: discovery of the complex radio emission from MACS J0717.5 +3745.
o	Table 2, Fig. 1-2: <[BFG2009] A> (Nos A-C, F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFG83]
[BFG83]	(Bechtold+Forman+Giacconi+, 1983)
Write:	<<[BFG83] pN>> <<[BFG83] eNN>> <<[BFG83] galaxy NN>>
N:	8+15+55
Object:	(X) + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	X-ray observations with the IPC and HRI aboard the Einstein Observatory. Table 2: found numbered in the literature, with format 'pN', (Nos p1-p8), letter 'p' for HRI Point source Table 4: found numbered in the literature, with format 'eNN', (Nos e1-e15), letter 'e' for Extended source Table 5: format 'galaxy NN', (Nos 1-55)
in source:	ACO 1367
Ref:	=1983ApJ...265...26B
by	BECHTOLD J. , FORMAN W., GIACCONI R., JONES C., SCHWARZ J., TUCKER W., VAN SPEYBROECK L.
	Astrophys. J., 265, 26-34 (1983)
	The X-ray morphology of Abell 1367.
o	Table 2: <[BFG83] pN> (Nos p1-p8), Table 4: <[BFG83] eNN> (Nos e1-e15), Table 5: <[BFG83] galaxy NN> (Nos 1-55)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFG97]
[BFG97]	(Boker+Forster-Schreiber+Genzel, 1997) (Not yet in Simbad)
Write:	<<[BFG97] Region N>>
N:	4
Object:	Region (SIMBAD class: PartofG = Part of a Galaxy)
in source:	IC 342
Ref:	=1997AJ....114.1883B
by	BOEKER T. , FOERSTER-SCHREIBER N.M., GENZEL R.
	Astron. J., 114, 1883-1898 (1997)
	Near-infrared imaging spectroscopy of IC 342: evolution of a bar-driven central starburst.
o	Table 2: <[BFG97] Region N> (Nos 1-4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFH91]
[BFH91]	(Beers+Forman+Huchra+, 1991)
Write:	<<[BFH91] HHMM+DDMMA>>
N:	534
Object:	G (SIMBAD class: Galaxy)
Note:	galaxies in the vicinity of 12 rich clusters: ACO 85, ACO 569, ACO 957, ACO 1069, ACO 1185, ACO 1750, ACO 1991, ACO 2063, ACO 2440, ACO 2589, ACO 2593, and ACO 2657
Ref:	=1991AJ....102.1581B
by	BEERS T.C. , FORMAN W., HUCHRA J.P., JONES C., GEBHARDT K.
	Astron. J., 102, 1581-1609 (1991)
	A dynamical analysis of twelve clusters of galaxies.
o	Table 1: <[BFH91] HHMM+DDMMA> N=534
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFJ2009]
[BFJ2009]	(Baldi+Forman+Jones+, 2009)
Write:	<<[BFJ2009] DN>> <<[BFJ2009] UN>>
N:	5+9
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS observations of the galaxy group AWM 5.
in source:	AWM 5
Ref:	=2009ApJ...694..479B
by	BALDI A. , FORMAN W., JONES C., NULSEN P., DAVID L., KRAFT R., SIMIONESCU A.
	Astrophys. J., 694, 479-491 (2009)
	Chandra observations of the galaxy group AWM 5: cool core reheating and thermal conduction suppression.
o	Table 2, Fig. 11: <[BFJ2009] DN> (Nos D1-D5), <[BFJ2009] UN> (Nos U1-U9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFK2002]
[BFK2002]	(Bachiller+Fuente+Kumar, 2002) (Not yet in Simbad)
Write:	<<[BFK2002] N>> <<[BFK2002] A>>
N:	5+1
Object:	* + Filament (SIMBAD class: Star)
Note:	N=5 near IR stars in RNO 6 region, and N=1 bright H2 filament 'F'.
Ref:	=2002A&A...381..168B
by	BACHILLER R. , FUENTE A., KUMAR M.S.N.
	Astron. Astrophys., 381, 168-177 (2002)
	Cometary molecular clouds around RNO6. On-going star formation near the double cluster h and χ Persei.
o	<NAME RNO 6 MCld>, <NAME RNO 6NW MCld>. Fig.2: <[BFK2002] N> (Nos 1-5), <[BFK2002] A> (No. F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFK2006]
[BFK2006]	(Brough+Forbes+Kilborn+, 2006)= (GEMS)
Note:	New group galaxies found in Parkes HI maps.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFK2008]
[BFK2008]	(Brassington+Fabbiano+Kim+, 2008)
Write:	<<[BFK2008] NNN>> <<[BFK2008] JHHMMSS.s+DDMMSS>>
N:	124
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS-S observations of NGC 3379.
in source:	NGC 3379
Ref:	=2008ApJS..179..142B
by	BRASSINGTON N.J. , FABBIANO G., KIM D.-W., ZEZAS A., ZEPF S., KUNDU A., ANGELINI L., DAVIES R.L., GALLAGHER J., KALOGERA V., FRAGOS T., KING A.R., PELLEGRINI S., TRINCHIERI G.
	Astrophys. J., Suppl. Ser., 179, 142-165 (2008)
	Deep Chandra monitoring observations of NGC 3379: catalog of source properties.
o	Table 4: <[BFK2008] NNN> (Nos 1-124) = <[BFK2008] JHHMMSS.s+DDMMSS> N=124.
=E=	Catalogue in electronic form as J/ApJS/179/142
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFK2009]
[BFK2009]	(Brassington+Fabbiano+Kim+, 2009)
Write:	<<[BFK2009] NNN>> <<[BFK2009] JHHMMSS.s+DDMMSS>>
N:	236
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS-S observations of NGC 4278.
in source:	NGC 4278
Ref:	=2009ApJS..181..605B
by	BRASSINGTON N.J. , FABBIANO G., KIM D.-W., ZEZAS A., ZEPF S., KUNDU A., ANGELINI L., DAVIES R.L., GALLAGHER J., KALOGERA V., FRAGOS T., KING A.R., PELLEGRINI S., TRINCHIERI G.
	Astrophys. J., Suppl. Ser., 181, 605-626 (2009)
	Deep Chandra monitoring observations of NGC 4278: catalog of source properties.
o	Table 3: <[BFK2009] NNN> (Nos 1-236) = <[BFK2009] JHHMMSS.s+DDMMSS> N=236.
=E=	Catalogue in electronic form as J/ApJS/181/605
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFK93]
[BFK93]	(Bonnet+Fort+Kneib+, 1993)
Write:	<<[BFK93] GN>> <<[BFK93] AN>> <<[BFK93] A2-N>> <<[BFK93] SN>> <<[BFK93] QNA>>
N:	7+3+4+3
Object:	G + Arc + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Observations of QSO 2345+007 field. N=3 galaxies, (Nos G1-G3). N=3 Arcs (LensedImage), (Nos A, B, D). N=4 arclets, (Nos A1-A4), 3 differents regions can be distinguished in arclet A2: (Nos A2-1 to A2-3). N=3 fields stars (Nos S1-S3). N=3 QSO, (Nos Q1A, Q1B, Q2). N=1 ClG J2348+0057, centered on C1.
Ref:	=1993A&A...280L...7B
by	BONNET H. , FORT B., KNEIB J.-P., MELLIER Y., SOUCAIL G.
	Astron. Astrophys., 280, 7-10 (1993)
	Detection of weak lensing by a massive dark halo in Q 2345+007.
o	Q1A = QSO 2345+007A, Q1B = QSO 2345+007B
o	Table 1, Fig. 1,2: <[BFK93] GN> (Nos G1-G2), <[BFK93] A> No. A, <[BFK93] AN> (Nos A1-A3), <[BFK93] SN> (Nos S1-S3), <[BFK93] QNA> (Nos Q1A, Q1B, Q2)
Ref:	=1994A&A...289L..15M
by	MELLIER Y. , DANTEL-FORT M., FORT B., BONNET H.
	Astron. Astrophys., 289, 15-18 (1994)
	Detection of a distant cluster in the center of the shear field in Q2345+007.
o	<[BFK93] A> (Nos B, D)
Ref:	=1996A&A...314...73P
by	PELLO R. , MIRALLES J.M., LE BORGNE J.-F., PICAT J.-P., SOUCAIL G., BRUZUAL G.
	Astron. Astrophys., 314, 73-86 (1996)
	Identification of a high redshift cluster in the field of Q2345+007 through deep BRIJK' photometry.
o	QA = QSO 2345+007A, QB = QSO 2345+007B
o	Fig. 1: <[BFK93] GN> (No. G3) added, <[BFK93] AN> (Nos C1, A4) added. Table 3: <[BFK93] A2-N> (Nos A2-1 to A2-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFM2002]
[BFM2002]	(Bernstein+Freedman+Madore, 2002)
Write:	<<[BFM2002] JHHMMSS.ss+DDMMSS.s>>
N:	140+687+644
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST WFPC2 observations: search for EBL sources (Extragalactic Background Light). Second author says: the objects should be refered as [BFM2003] JHHMMSS.ss+DDMMSS.s. See also EBL.
Ref:	=2002ApJ...571...56B
by	BERNSTEIN R.A. , FREEDMAN W.L., MADORE B.F.
	Astrophys. J., 571, 56-84 (2002)
	The first detections of the extragalactic background light at 3000, 5500, and 8000 Å. I. Results.
o	(Erratum) erratum vol. 632, p. 713 (2005)
o	Table 2: <EBL NNN-N-NNN> N=140+687+644 = <[BFM2002] JHHMMSS.ss-DDMMSS.s> N=140+687+644.
=E=	Catalogue in electronic form as J/ApJ/571/56
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BFM2004]
[BFM2004]	(Barlow+Fabbri+Meixner+, 2004)
Write:	<<[BFM2004] Star N>>
N:	5
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC observations and Gemini North follow-up mid-IR observations of NGC 6946. Detection of SN 2002HH and 4 other stars.
in source:	NGC 6946
Ref:	=2004IAUC.8400....2B
by	BARLOW M. , FABBRI J., MEIXNER M., SUGERMAN B.
	IAU Circ., 8400, 2-None (2004)
	Supernova 2002hh in NGC 6946.
o	<[BFM2004] Star N> (Nos 1-4).
Ref:	=2005ApJ...627L.113B
by	BARLOW M.J. , SUGERMAN B.E.K., FABBRI J., MEIXNER M., FISHER R.S., BOWEY J.E., PANAGIA N., ERCOLANO B., CLAYTON G.C., COHEN M., GLEDHILL T.M., GORDON K., TIELENS A.G.G.M., ZIJLSTRA A.A.
	Astrophys. J., 627, 113-116 (2005)
	Detection of a massive dust shell around the type II supernova SN 2002hh.
o	Table 1: <[BFM2004] Star N> (No. 5 added).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFO2002]
[BFO2002]	(Bellazzini+Ferraro+Origlia+, 2002)
Write:	<<[BFO2002] UMi NNNNN>> <<[BFO2002] Dra NNNNN>>
N:	4439+4586
Object:	* (SIMBAD class: Star)
Note:	TNG observations. Photometry of two wide fields centered on the dwarf speroidal galaxies Draco and Ursa Minor.
in source:	NAME UMi Dwarf Galaxy
in source:	NAME Draco Dwarf Galaxy
Ref:	=2002AJ....124.3222B
by	BELLAZZINI M. , FERRARO F.R., ORIGLIA L., PANCINO E., MONACO L., OLIVA E.
	Astron. J., 124, 3222-3240 (2002)
	The Draco and Ursa Minor dwarf spheroidal galaxies: a comparative study.
o	Table 1: <[BFO2002] UMi NNNNN> N=4439 among (Nos 10018 to 92168). Table 2: <[BFO2002] Dra NNNNN> N=4586 among (Nos 10069 to 91882).
=E=	Catalogue in electronic form as J/AJ/124/3222
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFO2013]
[BFO2013]	(Brosch+Finkelman+Oosterloo+, 2013)
Write:	<<[BFO2013] ON>>
N:	2
Object:	HI (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	WSRT HI observations of N=2 HI clouds near Hoag's Object.
Ref:	=2013MNRAS.435..475B
by	BROSCH N. , FINKELMAN I., OOSTERLOO T., JOZSA G., MOISEEV A.
	Mon. Not. R. Astron. Soc., 435, 475-481 (2013)
	HI in HO: Hoag's Object revisited.
o	Fig. 1, Table 1: <[BFO2013] ON> (Nos O1-O2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFO2019]
[BFO2019]	(Bentz+Ferrarese+Onken+, 2019)
Write:	<<[BFO2019] NN>>
N:	90
Object:	Poss. Cepheid (SIMBAD class: Cepheid_Candidate = Cepheid Variable Candidate)
Stat:	is completely incorporated in Simbad
Note:	HST WFC3 observations of N=90 Cepheid candidates in NGC 6814.
in source:	NGC 6814
Ref:	=2019ApJ...885..161B
by	BENTZ M.C. , FERRARESE L., ONKEN C.A., PETERSON B.M., VALLURI M.
	Astrophys. J., 885, 161-161 (2019)
	A Cepheid-based distance to the Seyfert galaxy NGC 6814.
o	Table 2: <[BFO2019] NN> (Nos 1-90).
=E=	Catalogue in electronic form as <J/ApJ/885/161/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFP2005]
[BFP2005]	(Bloom+Foley+Pooley+, 2005)
Write:	<<[BFP2005] JN>>
N:	5
Object:	* (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Keck I LRIS observations of the field of GRB 050509B.
Ref:	=2005GCN..3417....1B
by	BLOOM J.S. , FOLEY R.J., POOLEY D., FILIPPENKO A.V., CHORNOCK R., BLAKE C., PROCHASKA J.X., HENNAWI J., GLADDERS M., KOESTER B., CHEN H.W.
	GRB Coordinates Network, Circular Service, 3417, 1-None (2005)
	GRB 050509b: Keck/Chandra cross-correlation.
o	Text, Fig.: <[BFP2005] JN> (Nos J1-J4).
Ref:	=2006ApJ...638..354B
by	BLOOM J.S. , PROCHASKA J.X., POOLEY D., BLAKE C.H., FOLEY R.J., JHA S., RAMIREZ-RUIZ E., GRANOT J., FILIPPENKO A.V., SIGURDSSON S., BARTH A.J., CHEN H.-W., COOPER M.C., FALCO E.E., GAL R.R., GERKE B.F., GLADDERS M.D., GREENE J.E., HENNANWI J., HO L.C., HURLEY K., KOESTER B.P., LI W., LUBIN L., NEWMAN J., PERLEY D.A., SQUIRES G.K., WOOD-VASEY W.M.
	Astrophys. J., 638, 354-368 (2006)
	Closing in on a short-hard burst progenitor: constraints from early-time optical imaging and spectroscopy of a possible host galaxy of GRB 050509b.
o	Galaxy G1 = 2MASX J12361286+2858580
o	<[BFP2005] JN> (No. J5) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFR2003]
[BFR2003]	(Bally+Feigelson+Reipurth, 2003)
Write:	<<[BFR2003] NN>>
N:	69
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of the LDN 1551 molecular Cloud. [BFR2003] 31 is the source of X ray emission discovered by 2002A&A...386..204F.
in source:	LDN 1551
Ref:	=2003ApJ...584..843B
by	BALLY J. , FEIGELSON E., REIPURTH B.
	Astrophys. J., 584, 843-852 (2003)
	X-rays from the vicinity of the protostar L1551 IRS 5: reflection or fast shocks.
o	Table 1: <[BFR2003] NN> (Nos 1-69).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFR84]
[BFR84]	(Burns+Fitzferald+Reed, 1984) (Not yet in Simbad)
Write:	<<[BFR84] NNN>>
N:	130
Object:	* (SIMBAD class: Star)
Note:	Fig. 1: finding chart
Ref:	=1984MNRAS.206..327B
by	BURNS P.D. , FITZGERALD M.P., REED B.C.
	Mon. Not. R. Astron. Soc., 206, 327-336 (1984)
	Distribution of B5 to A5 stars at (l,b) = (253, -7).
o	Table 1: only 'HD NNNNN' are in Simbad
o	Table 1: <[BFR84] NNN> N=130 among (Nos 1-418)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BFS
BFS	(Blitz+Fich+Stark)= (B)
Write:	<<BFS NN>>
N:	65
Object:	HII + RFN (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	HII regions, not in Sharpless 1959 catalogue.
Ref:	=1982ApJS...49..183B
by	BLITZ L. , FICH M., STARK A.A.
	Astrophys. J., Suppl. Ser., 49, 183-206 (1982)
	Catalogue of CO radial velocities toward galactic HII regions.
o	Table B: <BFS NN> (Nos 1-65)
=E=	Catalogue in electronic form as VII/50
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BFS2001]
[BFS2001]	(Blair+Fesen+Schlegel, 2001) (Not yet in Simbad)
Write:	<<[BFS2001] Star a>> <<[BFS2001] Loop N>>
N:	4+3
Object:	* + Loop (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST observations of the field of [MF97] NGC 6946 16 SNR. N=4 brightest isolated stars, and N=3 features or Loops.
Ref:	=2001AJ....121.1497B
by	BLAIR W.P. , FESEN R.A., SCHLEGEL E.M.
	Astron. J., 121, 1497-1506 (2001)
	Hubble space telescope images of the ultraluminous supernova remnant complex in NGC 6946.
o	Fig.1, Table 2: <[BFS2001] Star a> (Nos a-d). Fig.5: <[BFS2001] Loop N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFS2004]
[BFS2004]	(Brown+Ferguson+Smith+, 2004)
Write:	<<[BFS2004] VNNN>>
N:	115 among 174
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	HST observations of M 31 Halo. N=55 RR Lyr, N=60 other V*.
in source:	M 31 = NGC 224
Ref:	=2004AJ....127.2738B
by	BROWN T.M. , FERGUSON H.C., SMITH E., KIMBLE R.A., SWEIGART A.V., RENZINI A., RICH R.M.
	Astron. J., 127, 2738-2752 (2004)
	RR Lyrae stars in the Andromeda halo from deep imaging with the advanced camera for surveys.
o	Tables 1, 3: <[BFS2004] VNNN> N=115 among (Nos V1-V174).
=E=	Catalogue in electronic form as J/AJ/127/2738
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFS2005]
[BFS2005]	(Beck+Fletcher+Shukurov+, 2005)
Write:	<<[BFS2005] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	rG (SIMBAD class: RadioG = Radio Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLA 3.5 and 6cm observations. A radio galaxy is found in the field of NGC 1097.
Ref:	=2005A&A...444..739B
by	BECK R. , FLETCHER A., SHUKUROV A., SNODIN A., SOKOLOFF D.D., EHLE M., MOSS D., SHOUTENKOV V.
	Astron. Astrophys., 444, 739-765 (2005)
	Magnetic fields in barred galaxies. IV. NGC 1097 and NGC 1365.
o	Paragr.3.1: <[BFS2005] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFS2016]
[BFS2016]	(Bernard+Ferguson+Schlafly+, 2016)= ([BFS2016a])
Write:	<<[BFS2016] PS1-A>>
N:	5
Object:	Poss. Stellar Stream (SIMBAD class: Stream = Stellar Stream)
Note:	N=5 candidate stellar streams discovered using the Pan-STARRS 3π Survey data set.
Ref:	=2016MNRAS.463.1759B
by	BERNARD E.J. , FERGUSON A.M.N., SCHLAFLY E.F., MARTIN N.F., RIX H.-W., BELL E.F., FINKBEINER D.P., GOLDMAN B., MARTINEZ-DELGADO D., SESAR B., WYSE R.F.G., BURGETT W.S., CHAMBERS K.C., DRAPER P.W., HODAPP K.W., KAISER N., KUDRITZKI R.-P., MAGNIER E.A., METCALFE N., WAINSCOAT R.J., WATERS C.
	Mon. Not. R. Astron. Soc., 463, 1759-1768 (2016)
	A Synoptic Map of Halo Substructures from the Pan-STARRS1 3π Survey.
o	Fig. 1, Table 1: <[BFS2016] PS1-A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFS2016a]
[BFS2016a]	(Bernard+Ferguson+Schlafly+, 2016)
*****	Avoid the usage of [BFS2016a], prefer [BFS2016]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFS2016b]
[BFS2016b]	(Bouche+Finley+Schroetter+, 2016)
Write:	<<[BFS2016b] objNNN>>
N:	41
Object:	G (SIMBAD class: Galaxy)
Stat.	in SIMBAD: Table 2: No 13 missing
Note:	VLT MUSE spectroscopic observations of N=41 galaxies at z∼0.91 in the field of SDSS J142253.31-000149.0 quasar.
in source:	SDSS J142253.31-000149.0
Ref:	=2016ApJ...820..121B
by	BOUCHE N. , FINLEY H., SCHROETTER I., MURPHY M.T., RICHTER P., BACON R., CONTINI T., RICHARD J., WENDT M., KAMANN S., EPINAT B., CANTALUPO S., STRAKA L.A., SCHAYE J., MARTIN C.L., PEROUX C., WISOTZKI L., SOTO K., LILLY S., CAROLLO C.M., BRINCHMANN J., KOLLATSCHNY W.
	Astrophys. J., 820, 121 (2016)
	Possible signatures of a cold-flow disk from MUSE using a z ~ 1 galaxy-quasar pair toward SDSS J1422-0001.
o	Table 2: <[BFS2016b] objNNN> N=41 among (Nos obj001-obj042).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFS2019]
[BFS2019]	(Bettoni+Falomo+Scarpa+, 2019) (Not yet in Simbad)
Write:	<<[BFS2019] J2211-0350 A>> <<[BFS2019] J2211-0350 Gal>> <<[BFS2019] J2211-0350 source>>
N:	4+1+1
Object:	Grav. lens system + Grav. lensed image + Galaxy (SIMBAD class: Optical = Optical Source)
Note:	Archival HST data combined with GTC OSIRIS spectroscopic observations of RXC J2211.7-0349 revealing a new Einstein cross.
in source:	RXC J2211.7-0350
Ref:	=2019ApJ...873L..14B
by	BETTONI D. , FALOMO R., SCARPA R., NEGRELLO M., OMIZZOLO A., CORRADI R.L.M., REVERTE D., VULCANI B.
	Astrophys. J., 873L, 14-14 (2019)
	A new Einstein Cross gravitational lens of a Lyman-break galaxy.
o	Table 1: <[BFS2019] J2211-0350 A> (Nos A to D), <[BFS2019] J2211-0350 Gal> N=1. Text: <[BFS2019] J2211-0350 source> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFS85]
[BFS85]	(Boyle+Fong+Shanks, 1985)
Write:	<<[BFS85] SGP ANN>> <<[BFS85] SGP AAN>> <<[BFS85] 22h ANN>> <<[BFS85] 22h AN.N>> <<[BFS85] 12h30 NNA>> <<[BFS85] 12h30 NNAN>> <<[BFS85] 12h30 NAA>>
N:	93
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	Table 3: (UV) in 3 fields: SGP, 22h, and 12h30
Ref:	=1985MNRAS.216..623B
by	BOYLE B.J. , FONG R., SHANKS T., CLOWES R.G.
	Mon. Not. R. Astron. Soc., 216, 623-639 (1985)
	A spectroscopic survey of faint ultraviolet excess stellar objects.
o	Table 3: <[BFS85] SGP ANN> (Nos S1-S20). <[BFS85] SGP ANN>, <[BFS85] SGP AAN> N=21. <[BFS85] 22h ANN> N=8 among (Nos T1-T31), <[BFS85] 22h AN.N> N=6. <[BFS85] 12h30 NNA>, <[BFS85] 12h30 NNAN>, <[BFS85] 12h30 NAN> N=28
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFS98]
[BFS98]	(Brown+Ferguson+Stanford+, 1998)
Write:	<<[BFS98] JHHMMSS.sss+DDMMSS.ss>>
N:	433+138
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Faint Object Camera (FOC) UV images of the 14"x14" of M 31 (N=433 stars) and M 32 (N=138 stars).
in source:	M 31 = NGC 224
in source:	M 33 = NGC 598
Ref:	=1998ApJ...504..113B
by	BROWN T.M. , FERGUSON H.C., STANFORD S.A., DEHARVENG J.M.
	Astrophys. J., 504, 113-138 (1998)
	Color-luminosity relations for the resolved hot stellar populations in the centers of M31 and M32.
o	Tables 2, 3: <[BFS98] JHHMMSS.sss+DDMMSS.ss> N=433+138.
=E=	Catalogue in electronic form as J/ApJ/504/113
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BFSP
BFSP	(Boyle+Fong+Shanks+Peterson)
*****	Avoid the usage of BFSP, prefer FOCAP
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BFT2007]
[BFT2007]	(Broos+Feigelson+Townsley+, 2007)= (ACIS)
Write:	<<[BFT2007] NNN>>
N:	886
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS observations of the stellar populations in and around M 17.
in source:	M 17 = NGC 6618
Ref:	=2007ApJS..169..353B
by	BROOS P.S. , FEIGELSON E.D., TOWNSLEY L.K., GETMAN K.V., WANG J., GARMIRE G.P., JIANG Z., TSUBOI Y.
	Astrophys. J., Suppl. Ser., 169, 353-385 (2007)
	The young stellar population in M17 revealed by Chandra.
o	Tables 1-2: <[BFT2007] NNN> (Nos 1-886).
=E=	Catalogue in electronic form as J/ApJS/169/353
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFT2010]
[BFT2010]	(Bielby+Finoguenov+Tanaka+, 2010)
Write:	<<[BFT2010] DDD.dddd+DD.dddd>>
N:	41
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=42 sources around N=6 WIRCam Deep Survey (WIRDS) cluster candidates (see WIRD). Use of CFHTLS deep optical data, WIRDS near-infrared data, and VVDS and AAT AAOmega spectroscopic data in the CFHTLS D1 and D4 fields.
Ref:	=2010A&A...523A..66B
by	BIELBY R.M. , FINOGUENOV A., TANAKA M., McCRACKEN H.J., DADDI E., HUDELOT P., ILBERT O., KNEIB J.P., LE FEVRE O., MELLIER Y., NANDRA K., PETITJEAN P., SRIANAND R., STALIN C.S., WILLOTT C.J.
	Astron. Astrophys., 523A, 66-66 (2010)
	The WIRCAM Deep Infrared Cluster Survey. I. Groups and clusters at z> 1.1.
o	Tables 3-4: <WIRD XC JHHMM.m+DDMM> N=9. Fig. 2, Table 11: <WIRD CS DF-pNNN> N=3. Tables 5-10: <[BFT2010] DDD.dddd+DD.dddd> N=41.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFT97]
[BFT97]	(Bernstein+Fischer+Tyson+, 1997)
Write:	<<[BFT97] G1>> <<[BFT97] Arc>> <<[BFT97] Knot N>> <<[BFT97] Blob N>>
N:	1+1+2+7
Object:	Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of the lensed double QSO 0957+561 and of sources in the vicinity of the QSO: N=1 galaxy 'G1' (= YGKOW G1), N=1 'Arc', N=2 substructures of the arc 'Knot 1' and 'Knot 2', and N=7 other sources called 'Blob 1 to Blob 7' by the authors. See also YGKOW, [RGH85], [GWC92], [BTK93], [ACL97], [BLF99], [PMN99], [SOS99], [TF99].
Ref:	=1997ApJ...483L..79B
by	BERNSTEIN G. , FISCHER P., TYSON J.A., RHEE G.
	Astrophys. J., 483, 79-82 (1997)
	Improved parameters and new lensed features for Q0957+561 from WFPC2 imaging.
o	Table 1: <[BFT97] G1>. Table 2: <[BFT97] Arc> N=1, <[BFT97] Knot N> (Nos 1-2), <[BFT97] Blob N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFV2003]
[BFV2003]	(Bloom+Fox+Van Dokkum+, 2003)
Write:	<<[BFV2003] JHHMMSS.ss+DDMMSS.s>> <<[BFV2003] JHHMMSS.sss+DDMMSS.ss>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Faint blue galaxies in the field of GRB 011030.
Ref:	=2003ApJ...599..957B
by	BLOOM J.S. , FOX D., VAN DOKKUM P.G., KULKARNI S.R., BERGER E., DJORGOVSKI S.G., FRAIL D.A.
	Astrophys. J., 599, 957-963 (2003)
	The first two host galaxies of X-ray flashes: XRF 011030 and XRF 020427.
o	note 12: <[BFV2003] JHHMMSS.ss+DDMMSS.s> N=2, <[BFV2003] JHHMMSS.sss+DDMMSS.ss> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFV2016]
[BFV2016]	(Brewer+Fischer+Valenti+, 2016)= (HTR)
Write:	<<[BFV2016] HTRFFF-NNNA>>
N:	93
Object:	* (SIMBAD class: Star)
Note:	N=93 HATNet TRansit candidates from the HATnet project. See also [LBT2009].
Ref:	=2016ApJS..225...32B
by	BREWER J.M. , FISCHER D.A., VALENTI J.A., PISKUNOV N.
	Astrophys. J., Suppl. Ser., 225, 32-32 (2016)
	Spectral properties of cool stars: extended abundance analysis of 1,617 planet-search stars.
o	Only known stars have been processed in SIMBAD; new objects have not been processed because of poor astrometry.
o	(Erratum) erratum vol. 230, art. 12 (2017)
o	Tables 8-9, 11: <SPOCS NNNN> (Nos 2000-3247) added. Tables 8-9, 11: <[BFV2016] HTRFFF-NNNA> N=93 among (Nos HTR056-003 to HTR433-003).
=E=	Catalogue in electronic form as <J/ApJS/225/32/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BFW2006]
[BFW2006]	(Berlind+Frieman+Weinberg+, 2006)
Write:	<<[BFW2006] MrNN NNNNN>> <<[BFW2006] MrNN NNNNN DDD.dddddd+DD.dddddd>>
N:	8148+113853
Object:	Group of G + G in Group (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Identification of N=4107+2684+1357 galaxy groups in volume-limited samples of the SDSS redshift survey. The three selected samples are complete down to absolute r-band magnitudes of M_r←19.9, -19, and -18, and are referred to as Mr20, Mr19, Mr18. Identification of N=57138+37820+18895 galaxies in these galaxy groups.
Ref:	=2006ApJS..167....1B
by	BERLIND A.A. , FRIEMAN J., WEINBERG D.H., BLANTON M.R., WARREN M.S., ABAZAJIAN K., SCRANTON R., HOGG D.W., SCOCCIMARRO R., BAHCALL N.A., BRINKMANN J., GOTT III J.R., KLEINMAN S.J., KRZESINSKI J., LEE B.C., MILLER C.J., NITTA A., SCHNEIDER D.P., TUCKER D.L., ZEHAVI I., (The SDSS Collaboration)
	Astrophys. J., Suppl. Ser., 167, 1-25 (2006)
	Percolation galaxy groups and clusters in the SDSS redshift survey: Identification, catalogs, and the multiplicity function.
o	Table 3: <[BFW2006] MrNN NNNNN> N=4107+2684+1357. Table 4: <[BFW2006] MrNN NNNNN DDD.dddddd-DD.dddddd> N=57138+37820+18895.
=E=	Catalogue in electronic form as J/ApJS/167/1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BFW78
BFW78	(Bohuski+Fairall+Weedman, 1978)
Write:	<<BFW78 NN>>
N:	90
Object:	EmG + QSO (SIMBAD class: Galaxy)
Note:	Table 1: (Nos 1-90), cross-id. with Tol HHMM.m+DD.d.
Ref:	=1978ApJ...221..776B
by	BOHUSKI T.J. , FAIRALL A.P., WEEDMAN D.W.
	Astrophys. J., 221, 776-787 (1978)
	The nature of Tololo emission-line galaxies.
o	Table 1, col (1): <BFW78 NN> (Nos 1-90) = Table 1, col (2): <Tol HHMM+DDd>, <Tol HHMM.m+DD.d> N=90.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BFZ2012]
[BFZ2012]	(Brassington+Fabbiano+Zezas+, 2012)
Write:	<<[BFZ2012] AN>>
N:	18 (SIMBAD class: X = X-ray Source)
Note:	Chandra X-ray observations of N=3 nearby elliptical galaxies. Search for transient sources.
in source:	NGC 3379
in source:	NGC 4278
in source:	NGC 4697
Ref:	=2012ApJ...755..162B
by	BRASSINGTON N.J. , FABBIANO G., ZEZAS A., KUNDU A., KIM D.-W., FRAGOS T., KING A.R., PELLEGRINI S., TRINCHIERI G., ZEPF S., WRIGHT N.J.
	Astrophys. J., 755, 162 (2012)
	The spectral and temporal properties of transient sources in early-type galaxies.
o	Table 2: <[BFZ2012] AN> (Nos A1-A8, B1-B8, C1-C2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BG
BG	(Bologna obs., Galactic)
Write:	<<BG HHMM+DDA>>
N:	586
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1974A&AS...16...43F
by	FANTI C. , FELLI M., FICARRA A., SALTER C.J., TOFANI G., TOMASI P.
	Astron. Astrophys., Suppl. Ser., 16, 43-61 (1974)
	1408MHz fan-beam survey at low galactic latitudes. I. The observations and a catalogue of small diameter sources.
o	<BG HHMM+DDA> or <BG HHMM+DDd> or <BG HHMM+DDNN> N=586
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BG
BG	(B. Gaston)
Write:	<<BG CFH NN>> <<BG KPN NN>>
N:	56+14
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	N=56 BG CFH (Canadian-France-Hawai tel.), N=14 BG KPN ( Kitt Peak National tel.).
Ref:	=1983ApJ...272..411G
by	GASTON B.
	Astrophys. J., 272, 411-433 (1983)
	Luminosity function of high-redshift quasars.
o	<BG CFH NN> (Nos 1-56), <BG KPN NN> (Nos 1-14).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BG
BG	(Block+Geballe+)
*****	Avoid the usage of BG, prefer [BGD93]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BG
BG	(Bok Globule)
*****	Avoid the usage of BG, prefer [GWC99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BG 57
BG 57	(B. Gaston, SA 57)
Write:	<<BG 57 NN>>
N:	54
Object:	QSO (SIMBAD class: QSO = Quasar)
Note:	In Veron+ 1984 (1984ESOSR...1....1V), format '57 NN', where '57' stands for 'SA 57', the ref. of B. Gaston for SA 57 has never been published, N=54 in Veron 1984.
Auth.:	GASTON B.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BG91]
[BG91]	(Bonnet-Bidaud+Gry, 1991)
Write:	<<[BG91] N>>
N:	9
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Brightest stars in a small field around Sirius. See also [BCL2000].
Ref:	=1991A&A...252..193B
by	BONNET-BIDAUD J.M. , GRY C.
	Astron. Astrophys., 252, 193-197 (1991)
	The stellar field in the vicinity of Sirius and the color enigma.
o	Table 1: <[BG91] N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGA2006]
[BGA2006]	(Burbidge+Gutierez+Arp, 2006)
Write:	<<[BGA2006] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations of the X-ray cluster RX J0152.7-1357: a blue optical and X-ray object is identified as a QSO.
Ref:	=2006PASP..118..124B
by	BURBIDGE E.M. , GUTIERREZ C.M., ARP H.
	Publ. Astron. Soc. Pac., 118, 124-128 (2006)
	A QSO discovered at the redshift of the extended X-ray cluster RX J0152.7-1357.
o	Text: <[BGA2006] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGB2001]
[BGB2001]	(Brandner+Grebel+Barba+, 2001)
Write:	<<[BGB2001] Naa>>
N:	8
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	HST NICMOS observations of 30 Dor nebula. Table 3: N= 8 objects, embedded in [WB87] knots 1 to 3. See also 30Dor-NIC.
in source:	Magellanic Clouds:LMC:30 Dor Nebula = 30 Dor Nebula
Ref:	=2001AJ....122..858B
by	BRANDNER W. , GREBEL E.K., BARBA R.H., WALBORN N.R., MONETI A.
	Astron. J., 122, 858-865 (2001)
	Hubble space telescope NICMOS detection of a partially embedded, intermediate-mass, pre-main-sequence population in the 30 Doradus nebula.
o	Table 3: 'Knot N' = '[WB87] N'. In Table 2, IRSN-134 is a misprint for IRSN-137 (cf. 2013AJ....145...98W).
o	Tables 1, 2: <30Dor-NIC NNa> N=24. Table 3: <[BGB2001] Naa> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGB2004]
[BGB2004]	(Boschin+Girardi+Barrena+, 2004)
Write:	<<[BGB2004] NNN>>
N:	132
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Data obtained at the Telescopio Nazionale Galileo (TNG) and from the CFHT archive. Velocity catalog of 132 spectroscopically measured galaxies in ACO 2219.
in source:	ACO 2219
Ref:	=2004A&A...416..839B
by	BOSCHIN W. , GIRARDI M., BARRENA R., BIVIANO A., FERETTI L., RAMELLA M.
	Astron. Astrophys., 416, 839-851 (2004)
	Internal dynamics of the radio-halo cluster A2219: A multi-wavelength analysis.
o	Table 1:<[BGB2004] NNN> (Nos 1-132).
=E=	Catalogue in electronic form as J/A+A/416/839
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGB2009]
[BGB2009]	(Barrena+Girardi+Boschin+, 2009)
Write:	<<[BGB2009] NNN>>
N:	145
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	TNG DOLORES/MOS spectroscopy and INT WFC photometry of the A1237+A1240 complex.
in source:	ACO 1240
Ref:	=2009A&A...503..357B
by	BARRENA R. , GIRARDI M., BOSCHIN W., DASI M.
	Astron. Astrophys., 503, 357-371 (2009)
	Internal dynamics of Abell 1240: a galaxy cluster with symmetric double radio relics.
o	Table 1: <[BGB2009] NNN> (Nos 1-145).
=E=	Catalogue in electronic form as J/A+A/503/357
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGB2011]
[BGB2011]	(Barrena+Girardi+Boschin+, 2011)
Write:	<<[BGB2011] NNN>>
N:	110
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	TNG DOLORES/MOS spectroscopy of N=110 galaxies in Abell 545.
in source:	ACO 545
Ref:	=2011A&A...529A.128B
by	BARRENA R. , GIRARDI M., BOSCHIN W., DE GRANDI S., ECKERT D., ROSSETTI M.
	Astron. Astrophys., 529A, 128-128 (2011)
	Internal dynamics of the galaxy cluster Abell 545. The ideal case where to study the simultaneous formation of a galaxy system and its brightest galaxy.
o	Table 1: <[BGB2011] NNN> (Nos 1-110).
=E=	Catalogue in electronic form as J/A+A/529/A128
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGB2012]
[BGB2012]	(Boschin+Girardi+Barrena+, 2012)= ([BGB2012a])
Write:	<<[BGB2012] NNN>>
N:	137
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	TNG DOLORES/MOS spectroscopy of N=137 galaxies in the field of the cluster Abell 1758N. Use of SDSS DR7 and CFHT archive.
in source:	NAME ACO 1758N
Ref:	=2012A&A...540A..43B
by	BOSCHIN W. , GIRARDI M., BARRENA R., NONINO M.
	Astron. Astrophys., 540A, 43-43 (2012)
	Abell 1758N from an optical point of view: new insights on a merging cluster with diffuse radio emission.
o	Table 1: <[BGB2012] NNN> (Nos 1-137).
=E=	Catalogue in electronic form as J/A+A/540/A43
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGB2012a]
[BGB2012a]	(Boschin+Girardi+Barrena+, 2012)
*****	Avoid the usage of [BGB2012a], prefer [BGB2012]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGB2012b]
[BGB2012b]	(Boschin+Girardi+Barrena, 2012)
Write:	<<[BGB2012b] NNN>>
N:	126
Object:	G (SIMBAD class: Galaxy)
Note:	TNG DOLORES spectroscopy and INT WFC photometry of N=126 galaxies in the field of the galaxy cluster Abell 1995.
in source:	ACO 1995
Ref:	=2012A&A...547A..44B
by	BOSCHIN W. , GIRARDI M., BARRENA R.
	Astron. Astrophys., 547A, 44-44 (2012)
	Structure of Abell 1995 from optical and X-ray data: a galaxy cluster with an elongated radio halo.
o	Table 1: <[BGB2012b] NNN> (Nos 1-126).
=E=	Catalogue in electronic form as J/A+A/547/A44
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGB2013]
[BGB2013]	(Barrena+Girardi+Boschin, 2013)= ([BGB2013a])
Write:	<<[BGB2013] NNN>>
N:	119
Object:	G (SIMBAD class: Galaxy)
Note:	TNG DOLORES spectroscopy of N=119 galaxies in the galaxy cluster Abell 1914.
in source:	ACO 1914
Ref:	=2013MNRAS.430.3453B
by	BARRENA R. , GIRARDI M., BOSCHIN W.
	Mon. Not. R. Astron. Soc., 430, 3453-3464 (2013)
	The puzzling merging cluster Abell 1914: new insights from the kinematics of member galaxies.
o	Table 1: <[BGB2013] NNN> (Nos 1-119).
o	400d J1425+3758 is [BVH2007] 5-10 in Simbad.
=E=	Catalogue in electronic form as <J/MNRAS/430/3453/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGB2013a]
[BGB2013a]	(Barrena+Girardi+Boschin, 2013)
*****	Avoid the usage of [BGB2013a], prefer [BGB2013]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGB2013b]
[BGB2013b]	(Boschin+Girardi+Barrena, 2013)
Write:	<<[BGB2013b] NNN>>
N:	128
Object:	G (SIMBAD class: Galaxy)
Note:	TNG DOLORES spectroscopy of N=128 galaxies in the galaxy cluster ZwCl 2341+0000.
in source:	ZwCl 2341+0000
Ref:	=2013MNRAS.434..772B
by	BOSCHIN W. , GIRARDI M., BARRENA R.
	Mon. Not. R. Astron. Soc., 434, 772-783 (2013)
	The dynamical status of ZwCl 2341.1+0000: a very elongated galaxy structure with a complex radio emission.
o	Table 1: <[BGB2013b] NNN> (Nos 1-128).
=E=	Catalogue in electronic form as <J/MNRAS/434/772/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGB2014]
[BGB2014]	(Barrena+Girardi+Boschin+, 2014)
Write:	<<[BGB2014] NNN>>
N:	135
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	TNG Multi-object spectroscopic (MOS) observations of N=135 galaxies in Abell 1351 cluster.
in source:	ACO 1351
Ref:	=2014MNRAS.442.2216B
by	BARRENA R. , GIRARDI M., BOSCHIN W., DE GRANDI S., ROSSETTI M.
	Mon. Not. R. Astron. Soc., 442, 2216-2227 (2014)
	The structure of Abell 1351: a bimodal galaxy cluster with peculiar diffuse radio emission.
o	BCG1 = 2MASX J11422472+5832048, BCG2 = 2MASX J11422626+5832428.
o	Table 1: <[BGB2014] NNN> (Nos 1-135).
=E=	Catalogue in electronic form as J/MNRAS/442/2216
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGB2018]
[BGB2018]	(Bitsakis+Gonzalez-Lopezlira+Bonfini+, 2018)
Write:	<<[BGB2018] SMC-IR1-NNN>> <<[BGB2018] SMC-M2-NNN>> <<[BGB2018] SMC-NUV-NNNN>>
N:	1319
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	N=1319 star clusters in the Small Magellanic Cloud. Use of archival data from GALEX, SUMAC survey (Swift/UVOT Magellanic Clouds Survey), MCPS survey (Magellanic Cloud Photometric Survey), and Spitzer MIPS. See also [BBG2017].
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2018ApJ...853..104B
by	BITSAKIS T. , GONZALEZ-LOPEZLIRA R.A., BONFINI P., BRUZUAL G., MARAVELIAS G., ZARITSKY D., CHARLOT S., RAMIREZ-SIORDIA V.H.
	Astrophys. J., 853, 104-104 (2018)
	The distribution and ages of star clusters in the Small Magellanic Cloud: constraints on the interaction history of the Magellanic Clouds.
o	Table 1: <[BGB2018] SMC-IR1-NNN> N=466 among (Nos IR1-182 to IR1-787), <[BGB2018] SMC-M2-NNN> N=453 among (Nos M2-1 to M2-455), <[BGB2018] SMC-NUV-NNNN> N=400 among (Nos NUV-480 to NUV-1091).
=E=	Catalogue in electronic form as J/ApJ/853/104
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGB98]
[BGB98]	(Boyle+Georgantopoulos+Blair+, 1998)
Write:	<<[BGB98] JHHMMSS.s+DDMMSSA>>
N:	34
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 1, col(3): N=34 possible optical counterpart to N=26 ASCA X-ray sources. the format is the optical position, 2 objects have the same optical position, so they are with a letter A and B at the end of the format. See also Paper I 1997MNRAS.291..203G.
Ref:	=1998MNRAS.296....1B
by	BOYLE B.J. , GEORGANTOPOULOS I., BLAIR A.J., STEWART G.C., GRIFFITHS R.E., SHANKS T., GUNN K.F., ALMAINI O.
	Mon. Not. R. Astron. Soc., 296, 1-9 (1998)
	ASCA observations of deep ROSAT fields - II. The 2-10 keV AGN luminosity function.
o	Table 1, col(3): <[BGB98] JHHMMSS.s-DDMMSSA> N=34.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGB99]
[BGB99]	(Brotherton+Gregg+Becker+, 1999)
Write:	<<[BGB99] J1643+3156 A>>
N:	2
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	Discovery of a QSO pair associated with the radio-source FIRST J164311.3+315618. The brightest quasar is 'J1643+3156 A', the pair is the lowest redshift and the smallest separation binary quasar yet identified.
in source:	FIRST J164311.0+315618
Ref:	=1999ApJ...514L..61B
by	BROTHERTON M.S. , GREGG M.D., BECKER R.H., LAURENT-MUEHLEISEN S.A., WHITE R.L., STANFORD S.A.
	Astrophys. J., 514, 61-64 (1999)
	Discovery of a radio-loud/radio-quiet binary quasar.
o	Table 1: <[BGB99] J1643+3156 A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BGC
BGC	(Burnham obs., General Catalog)
*****	Avoid the usage of BGC, prefer BDS
Details on Acronym: BGC
BGC	(Boss, General Catalog)
Note:	On magnetic tape.
*****	Avoid the usage of BGC, prefer GC
Origin	of the Acronym: L (1921LicOB..10..110T)
Details on Acronym: [BGC2000]
[BGC2000]	(Brandner+Grebel+Chu+, 2000)= (Proplyd)
Write:	<<[BGC2000] Proplyd N>>
N:	3
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 and VLT ISAAC observations of Orion nebula. N=3 'Proplyds' (Proto Planetary Disk) in Orion.
in source:	NAME Orion Nebula
Ref:	=2000AJ....119..292B
by	BRANDNER W. , GREBEL E.K., CHU Y.-H., DOTTORI H., BRANDL B., RICHLING S., YORKE H.W., POINTS S.D., ZINNECKER H.
	Astron. J., 119, 292-301 (2000)
	HST/WFPC2 and VLT/ISAAC observations of proplyds in the giant H II region NGC 3603.
o	Table 1: <[BGC2000] Proplyd N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BGD
BGD	(Block+Geballe+Dyson)
*****	Avoid the usage of BGD, prefer [BGD93]
Origin	of the Acronym: L (2003A&A...397..177B)
Details on Acronym: [BGD93]
[BGD93]	(Block+Geballe+Dyson, 1993)= (BG) = (BGD) = (IRS)
Write:	<<[BGD93] IRS N>>
N:	5
Object:	(IR) (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
in source:	NAME Rosette Molecular Cloud
Ref:	=1993A&A...273L..41B
by	BLOCK D.L. , GEBALLE T.R., DYSON J.E.
	Astron. Astrophys., 273, 41-43 (1993)
	An embedded cluster of stars at the Rosette GMC CO peak.
o	Table 1: <[BGD93] IRS N> (Nos 1-5)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGD98]
[BGD98]	(Bica+Geisler+Dottori+, 1998) (Not yet in Simbad)
Write:	<<[BGD98] SL NNN NNNNN>> <<[BGD98] IC 2134 NNNNN>> <<[BGD98] ESO 121-3 NNNN>> <<[BGD98] OHSC NN NNNNN>>
N:	1788
Object:	* in Cl* (SIMBAD class: Star)
Note:	N=1788 stars in 13 star clusters in the LMC.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1998AJ....116..723B
by	BICA E. , GEISLER D., DOTTORI H., CLARIA J.J., PIATTI A.E., SANTOS J.F.C.Jr
	Astron. J., 116, 723-737 (1998)
	Ages and metallicities of star clusters and surrounding fields in the outer disk of the Large Magellanic Cloud.
o	Table 2: <[BGD98] SL NNN NNNNN>, <[BGD98] IC 2134 NNNNN>, <[BGD98] ESO 121-3 NNNN>, <[BGD98] OHSC NN NNNNN>. N=1788.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BGE
BGE	(Bologna obs., Galactic, Extended)
Write:	<<BGE HHMM+DD>>
N:	77
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	15deg<L<245d, \|b\|<3.5deg. resol. 4.2'x1.9deg.
Ref:	=1977A&AS...27..181F
by	FELLI M. , TOFANI G., FANTI C., TOMASI P.
	Astron. Astrophys., Suppl. Ser., 27, 181-204 (1977)
	A 408 MHz fan-beam survey at low galactic latitudes. III. The catalogue of extended sources.
o	Table 1: <BGE HHMM+DD> N=77
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BGE2002]
[BGE2002]	(Beltran+Girart+Estalella+, 2002)= (BIMA) = (VLA)
Write:	<<[BGE2002] VLA N>> <<[BGE2002] BIMA NW>> <<[BGE2002] Clump A>>
N:	5+3+1+2
Object:	(Rad) + (mm) + Clump (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Centimeter observations of gas and dust around IRAS 21391+5802 embedded in the core of IC 1396N. N=5 VLA sources. N=3 BIMA (Berkeley-Illinois-Maryland Assoc.) mm sources (Nos 1-3), and a yet undetected YSO 'BIMA 1W'. N=2 CS emission clumps, B (blueshifted) and R (Redshifted).
in source:	IC 1396N
Ref:	=2002ApJ...573..246B
by	BELTRAN M.T. , GIRART J.M., ESTALELLA R., HO P.T.P., PALAU A.
	Astrophys. J., 573, 246-259 (2002)
	IRAS 21391+5802: the molecular outflow and its exciting source.
o	p. 247 : Calibrator 2148+611 not identified
o	Table 2: <[BGE2002] VLA N> (Nos 1-5). Table 3: <[BGE2002] BIMA N> (Nos 1-3). Fig.6: <[BGE2002] Clump A> (Nos B, R).
Ref:	=2004A&A...426..941B
by	BELTRAN M.T. , GIRART J.M., ESTALELLA R., HO P.T.P.
	Astron. Astrophys., 426, 941-949 (2004)
	The dense molecular cores in the IRAS 21391+5802 region.
o	Text: <[BGE2002] BIMA 1W> added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGE2005]
[BGE2005]	(Bastian+Gieles+Efremov+, 2005)
Write:	<<[BGE2005] AN>>
N:	4+7
Object:	Star Cluster Complex (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST WFPC2 and ACS observations of M 51: Search for young star cluster complexes in the spiral arms. See also [BGG2008].
in source:	M 51 = NGC 5194
Ref:	=2005A&A...443...79B
by	BASTIAN N. , GIELES M., EFREMOV Y.N., LAMERS H.J.G.L.M.
	Astron. Astrophys., 443, 79-90 (2005)
	Hierarchical star formation in M51: star/cluster complexes.
o	Table 1, Fig.1: <[BGE2005] AN> (Nos A1-D1, A2-G2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGE2006]
[BGE2006]	(Beltran+Girart+Estalella, 2006)= (OVRO)
Write:	<<[BGE2006] OVRO N>>
N:	4
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Owen Valley Radio Observatory (OVRO) 2.7 mm observations of LDN 1206.
in source:	LDN 1206
Ref:	=2006A&A...457..865B
by	BELTRAN M.T. , GIRART J.M., ESTALELLA R.
	Astron. Astrophys., 457, 865-876 (2006)
	Who is eating the outflow? High-angular resolution study of an intermediate-mass protostar in L1206.
o	Table 2: <[BGE2006] OVRO N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BGEM
BGEM	(BlackGEM)
Write:	<<BGEM JHHMMSS.ss+DDMMSS.s>>
N:	>1 billion
Object:	Star + Galaxy
Note:	The BlackGEM project is an array of wide-field optical telescopes, installed at the ESO La Silla Observatory. The prime scientific purpose of BlackGEM is the discovery of gravitational wave counterparts. It will also perform a Southern All Sky Survey (Dec<+30d) down to 22nd magnitude in all six filter bands (Sloan u,g,r,i,z + wide-band q) and a local universe (d<100 Mpc) transient program as well as deep drilling fields. It will be installed at La Silla in Q2 2019. http://www.blackgem.org @BlackGEM_Array on Twitter
Notes:	Positions are on the Gaia DR2 frame and are ICRS coordinates.
Auth.:	Paul Groot Radboud University / University of Cape Town
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [BGF2001]
[BGF2001]	(Brown+Geller+Fabricant+, 2001)= (cs)
Write:	<<[BGF2001] cs NNNN>>
N:	1295
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Brightest G in the Century Survey (cs in the format). Numbering under 3000 are galaxies listed in the original Century Survey described in 1997AJ....114.2205G See also [WTK2001].
Ref:	=2001AJ....122..714B
by	BROWN W.R. , GELLER M.J., FABRICANT D.G., KURTZ M.J.
	Astron. J., 122, 714-728 (2001)
	V- and R-band galaxy luminosity functions and low surface brightness galaxies in the Century Survey.
o	Table 3: < [BGF2001] cs NNNN> N=1295 among (Nos 2-1376 and 3002-3346).
=E=	Catalogue in electronic form as J/AJ/122/714
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGF2005]
[BGF2005]	(Bellazzini+Gennari+Ferraro, 2005)
Write:	<<[BGF2005] NNNN>>
N:	2716
Object:	* (SIMBAD class: Star)
Note:	TNG observations of a field centered on Leo II. See also [SM2000]
in source:	UGC 6253 = Leo II
Ref:	=2005MNRAS.360..185B
by	BELLAZZINI M. , GENNARI N., FERRARO F.R.
	Mon. Not. R. Astron. Soc., 360, 185-193 (2005)
	The red giant branch tip and bump of the Leo II dwarf spheroidal galaxy.
o	Catalogue: <[BGF2005] NNNN> N=2716 among (Nos 5-5432). Catalogue: <[SM2000] VNNN> (No. V173) added.
=E=	Catalogue in electronic form as J/MNRAS/360/185
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGF2006]
[BGF2006]	(Branchesi+Gioia+Fanti+, 2006)= (NEP)
Write:	<<[BGF2006] NEP NNNN>> <<[BGF2006] NEP NNNN A>>
N:	18+79
Object:	Cluster of G + (Rad) (SIMBAD class: Radio = Radio Source)
Note:	X-ray selected clusters of galaxies (format 'NEP NNNN' from an internal NEP ID) belonging to the ROSAT NEP survey are observed with the VLA at 1.4GHz: 79 radio sources are found in 17 of the clusters.
in source:	NAME NEP
Ref:	=2006A&A...446...97B
by	BRANCHESI M. , GIOIA I.M., FANTI C., FANTI R., PERLEY R.
	Astron. Astrophys., 446, 97-111 (2006)
	The radio luminosity function of the NEP distant cluster radio galaxies.
o	Table 1: RX J1812.1+6447 is a misprint for RX J1812.1+6353
o	Table 1: <[BGF2006] NEP NNNN> N=18 among (Nos 200-5281). Table 2: <[BGF2006] NEP NNNN A> N=79.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGF2007]
[BGF2007]	(Branchesi+Gioia+Fanti+, 2007)
Write:	<<[BGF2007] ACO 2125 NN>> <<[BGF2007] ClG HHMM+DDMM NN>> <<[BGF2007] ClG JHHMM+DDMM NN>>
N:	25+93
Object:	(X) in ClG (SIMBAD class: X = X-ray Source)
Note:	Chandra point sources in 18 distant galaxy clusters.
Ref:	=2007A&A...462..449B
by	BRANCHESI M. , GIOIA I.M., FANTI C., FANTI R., CAPPELLUTI N.
	Astron. Astrophys., 462, 449-458 (2007)
	Chandra point-source counts in distant galaxy clusters.
o	Table 2: <[BGF2007] ACO 2125 NN> (Nos 1-25), <[BGF2007] ClG HHMM+DDMM NN>, <[BGF2007] ClG JHHMM+DDMM NN>, N=93.
=E=	Catalogue in electronic form as J/A+A/462/449
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGF2009]
[BGF2009]	(Bonafede+Giovannini+Feretti+, 2009)
Write:	<<[BGF2009] ACO 2345-N>> <<[BGF2009] ACO 2345-N A>> <<[BGF2009] ACO 2345-XN>> <<[BGF2009] ACO 1240-N>> <<[BGF2009] ACO 1240-N A>> <<[BGF2009] JHHMMSSss+DDMMSSs>>
Object:	(Radio) (SIMBAD class: Radio = Radio Source)
Note:	VLA 20 and 90cm continuum observations of ACO 2345 and ACO 1240 .
in source:	ACO 2345
in source:	ACO 1240
Ref:	=2009A&A...494..429B
by	BONAFEDE A. , GIOVANNINI G., FERETTI L., GOVONI F., MURGIA M.
	Astron. Astrophys., 494, 429-442 (2009)
	Double relics in Abell 2345 and Abell 1240. Spectral index and polarization analysis.
o	Table 1: <[BGF2009] ACO 2345-N> (Nos 1-2), <[BGF2009] ACO 1240-N> (Nos 1-2). Fig. 1: <[BGF2009] ACO 2345-2 A> (Nos A-F), <[BGF2009] ACO 2345-1 A> (No. G). Fig. 4: <[BGF2009] ACO 2345 XN> (Nos X1-X3). Fig. 6: <[BGF2009] ACO 1240-1 A> (Nos A to C). Text: <[BGF2009] J21263466-1207214>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGF2020]
[BGF2020]	(Bally+Ginsburg+Forbrich+, 2020)
Write:	<<[BGF2020] SWN>> <<[BGF2020] EN>>
N:	4+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	JVLA 6GHz observations of N=4+2 radio sources in the field of the BN Object.
Ref:	=2020ApJ...889..178B
by	BALLY J. , GINSBURG A., FORBRICH J., VARGAS-GONZALEZ J.
	Astrophys. J., 889, 178-178 (2020)
	The Orion protostellar explosion and runaway stars revisited: stellar masses, disk retention, and an outflow from the Becklin-Neugebauer object.
o	Fig. 4, Tables 2+4+5: <[BGF2020] SWN> (Nos SW1-SW4), <[BGF2020] EN> (Nos E1-E2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BGG
BGG	(Bilkina+Getov+Georgiev)
Write:	<<BGG NNN>>
N:	104
Object:	* (SIMBAD class: Star)
Note:	* in the field of M 81
in source:	M 81 = NGC 3031
Ref:	=1991SoSAO..67..119B
by	BILKINA B.I. , GETOV R.G., GEORGIEV T.B.
	Soobshch. Spets. Astrof. Obs., 67, 119-128 (1991)
	A survey of blue and red stars in the field of 30'x30' around the M 81 galaxy.
o	<BGG NNN> N=104 among (Nos 1-296)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BGG2006]
[BGG2006]	(Brogan+Gelfand+Gaensler+, 2006)
Write:	<<[BGG2006] GLL.ll+B.bb>>
N:	35
Object:	Poss. SNR (SIMBAD class: SNRemnant_Candidate = SuperNova Remnant Candidate)
Stat:	is completely incorporated in Simbad
Note:	VLA survey of the Galactic Plane: discovery of 35 candidate SNRs.
Ref:	=2006ApJ...639L..25B
by	BROGAN C.L. , GELFAND J.D., GAENSLER B.M., KASSIM N.E., LAZIO T.J.W.
	Astrophys. J., 639, 25-29 (2006)
	Discovery of 35 new supernova remnants in the inner Galaxy.
o	Table 1: <[BGG2006] GLL.ll+B.bb> N=35.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGG2008]
[BGG2008]	(Bastian+Gieles+Goodwin+, 2008)
Write:	<<[BGG2008] aN>> <<[BGG2008] 3cl-a>> <<[BGG2008] G2a>>
N:	6
Object:	Stellar Cluster (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Gemini-North GMOS and HST ACS observations of M 51. See also [BGE2005].
in source:	M 51 = NGC 5194
Ref:	=2008MNRAS.389..223B
by	BASTIAN N. , GIELES M., GOODWIN S.P., TRANCHO G., SMITH L.J., KONSTANTOPOULOS I., EFREMOV Y.
	Mon. Not. R. Astron. Soc., 389, 223-230 (2008)
	The early expansion of cluster cores.
o	Table 1: <[BGG2008] aN> (No. a1), <[BGG2008] 3cl-a> (Nos 3cl-a to 3cl-c), <[BGG2008] G2a> (Nos G2a, G2b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGG2011]
[BGG2011]	(Bruevich+Gusev+Guslyakova, 2011)= ([BGG2011a])
Write:	<<[BGG2011] NGC 5585 NN>> <<[BGG2011] IC 1525 NN>>
N:	47+16
Object:	Star Forming Region (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Maidanak Observatory 1.5-m telescope UBVRI photometry of N=47+16 star-forming regions in NGC 5585 and IC 1525.
in source:	NGC 5585
in source:	IC 1525
Ref:	=2011ARep...55..310B
by	BRUEVICH V.V. , GUSEV A.S., GUSLYAKOVA S.A.
	ARep, 55, 310-323 (2011)
	Star-forming regions in the ring galaxies NGC 5585 and IC 1525.
o	Tables 2-3: <[BGG2011] NGC 5585 NN> (Nos 1-47), <[BGG2011] IC 1525 NN> (Nos 1-16).
o	2011AZh....88..342B
=E=	Catalogue in electronic form as J/AZh/88/342
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGG2011a]
[BGG2011a]	(Bruevich+Gusev+Guslyakova, 2011)
*****	Avoid the usage of [BGG2011a], prefer [BGG2011]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGG2011b]
[BGG2011b]	(Boutsia+Grazian+Giallongo+, 2011)
Write:	<<[BGG2011b] NNNNN>>
N:	45
Object:	LBG (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	LBT LBC deep UV observations of N=45 Lyman break galaxies at z=3.3.
Ref:	=2011ApJ...736...41B
by	BOUTSIA K. , GRAZIAN A., GIALLONGO E., FONTANA A., PENTERICCI L., CASTELLANO M., ZAMORANI G., MIGNOLI M., VANZELLA E., FIORE F., LILLY S.J., GALLOZZI S., TESTA V., PARIS D., SANTINI P.
	Astrophys. J., 736, 41 (2011)
	A low escape fraction of ionizing photons of l > l Lyman break* galaxies at z = 3.3.
o	Table 1: <[BGG2011b] NNNNN> N=11 among (Nos 1723-74113).
Ref:	=2016A&A...585A..48G
by	GRAZIAN A. , GIALLONGO E., GERBASI R., FIORE F., FONTANA A., LE FEVRE O., PENTERICCI L., VANZELLA E., ZAMORANI G., CASSATA P., GARILLI B., LE BRUN V., MACCAGNI D., TASCA L.A.M., THOMAS R., ZUCCA E., AMORIN R., BARDELLI S., CASSARA L.P., CASTELLANO M., CIMATTI A., CUCCIATI O., DURKALEC A., GIAVALISCO M., HATHI N.P., ILBERT O., LEMAUX B.C., PALTANI S., RIBEIRO B., SCHAERER D., SCODEGGIO M., SOMMARIVA V., TALIA M., TRESSE L., VERGANI D., BONCHI A., BOUTSIA K., CAPAK P., CHARLOT S., CONTINI T., DE LA TORRE S., DUNLOP J., FOTOPOULOU S., GUAITA L., KOEKEMOER A., LOPEZ-SANJUAN C., MELLIER Y., MERLIN E., PARIS D., PFORR J., PILO S., SANTINI P., SCOVILLE N., TANIGUCHI Y., WANG P.W.
	Astron. Astrophys., 585A, 48-48 (2016)
	The Lyman continuum escape fraction of galaxies at z = 3.3 in the VUDS-LBC/COSMOS field.
o	Table 1: <[BGG2011b] NNNNN> N=34 among (Nos 1723-74113) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGG2012]
[BGG2012]	(Barnard+Galache+Garcia+, 2012)
Write:	<<[BGG2012] NN>>
N:	14
Object:	X-ray Transient (SIMBAD class: Transient = Transient Event)
Stat:	is completely incorporated in Simbad
Note:	N=12 X-ray transients found in multi-epoch Chandra ACIS data.
in source:	M 31
Ref:	=2012ApJ...756...32B
by	BARNARD R. , GALACHE J.L., GARCIA M.R., NOORAEE N., CALLANAN P.J., ZEZAS A., MURRAY S.S.
	Astrophys. J., 756, 32 (2012)
	A period distribution of X-ray binaries observed in the central region of M31 with Chandra and the Hubble space telescope.
o	Table 2: <[BGG2012] NN> (Nos 1-12)
Ref:	=2014ApJ...780..169B
by	BARNARD R. , GARCIA M.R., PRIMINI F., MURRAY S.S.
	Astrophys. J., 780, 169 (2014)
	Discovery of a new black hole transient within 100'' (400 pc) of M31.*
o	Fig. 2, 4: <[BGG2012] NN> (No 13) added.
Ref:	=2015MNRAS.449.3426B
by	BARNARD R. , GARCIA M.R., MURRAY S.S.
	Mon. Not. R. Astron. Soc., 449, 3426-3431 (2015)
	Chandra, XMM-Newton and HST observations of a transient in M31 with a possible asymmetric, precessing disc.
o	Fig. 1: <[BGG2012] NN> (No 14) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BGH
BGH	(Beers+Geller+Huchra)
*****	Avoid the usage of BGH, prefer [BGH82]
Origin	of the Acronym: L (2000AJ....120.2269P)
Details on Acronym: [BGH2000]
[BGH2000]	(Blanton+Gregg+Helfand+, 2000)
Write:	<<[BGH2000] JHHMM+DDMM NN>>
N:	183
Object:	G (SIMBAD class: Galaxy)
Note:	Keck slit mask spectroscopic observations. Galaxies in 10 fields, each with a radio-source tracer for a cluster of galaxies. Maps in figs 1.
in source:	ClG J0221-0202
in source:	ClG J0320-0049
in source:	ClG J0730+2328
in source:	ClG J0819+2522
in source:	ClG J0910+3841
in source:	ClG J1119+3750
in source:	ClG J1209+2848
in source:	ClG J1234+4012
in source:	ClG J1338+2931
in source:	ClG J1418+3211
Ref:	=2000ApJ...531..118B
by	BLANTON E.L. , GREGG M.D., HELFAND D.J., BECKER R.H., WHITE R.L.
	Astrophys. J., 531, 118-136 (2000)
	FIRST bent-double radio sources: tracers of high-redshift clusters.
o	in ref list Gioia 1990ApJ...356L..35G instead of 356.35
o	Tables 4, 5: <[BGH2000] JHHMM+DDMM NN> N=183.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGH2001]
[BGH2001]	(Blanton+Gregg+Helfand+, 2001)
Write:	<<[BGH2001] NNN>>
N:	40
Object:	rG (SIMBAD class: RadioG = Radio Galaxy)
Note:	N=40 radio glaxies among 384 FIRST sources that exhibit the bent-double morphology. Maps in Fig.1.
Ref:	=2001AJ....121.2915B
by	BLANTON E.L. , GREGG M.D., HELFAND D.J., BECKER R.H., LEIGHLY K.M.
	Astron. J., 121, 2915-2927 (2001)
	The environments of a complete moderate-redshift sample of FIRST bent-double radio sources.
o	Tables 1, 2: <[BGH2001] NNN> N=40 among 384.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGH2003]
[BGH2003]	(Blanton+Gregg+Helfand+, 2003)
Write:	<<[BGH2003] A>> <<[BGH2003] NN>>
N:	10
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Table 1: spectroscopically confirmed galaxy members of the ClG J1137+3000. A is the radio host galaxy.
in source:	ClG J1137+3000
Ref:	=2003AJ....125.1635B
by	BLANTON E.L. , GREGG M.D., HELFAND D.J., BECKER R.H., WHITE R.L.
	Astron. J., 125, 1635-1641 (2003)
	Discovery of a high-redshift (z=0.96) cluster of galaxies using a FIRST survey wide-angle-tailed radio source.
o	Cluster = ClG J1137+3000
o	Table 1, Fig.4: <[BGH2003] A> (Nos A-C), <[BGH2003] NN> N=7 among (Nos 2-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGH82]
[BGH82]	(Beers+Geller+Huchra, 1982)= (BGH)
Write:	<<[BGH82] NNN>>
N:	28
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	See also [PBL2000].
in source:	ACO 98
Ref:	=1982ApJ...257...23B
by	BEERS T.C. , GELLER M.J., HUCHRA J.P.
	Astrophys. J., 257, 23-32 (1982)
	Galaxy clusters with multiple components. I. The dynamics of Abell 98.
o	Table 1: <[BGH82] NNN> N=28 among (Nos 30-422).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGH92]
[BGH92]	(Beers+Gebhardt+Huchra+, 1992)= ([BGH92a])
Write:	<<[BGH92] HHMM+DDMMA>> <<[BGH92] NN>>
N:	107
Object:	G in ClG (SIMBAD class: Galaxy)
Note:	Table 1, col (1): format 'HHMM+DDMMA', N=107 Table 1, col (2): format 'NN', N=99, cross-id. with format in col. (1)
in source:	ACO 400
Ref:	=1992ApJ...400..410B
by	BEERS T.C. , GEBHARDT K., HUCHRA J.P., FORMAN W., JONES C., BOTHUN G.D.
	Astrophys. J., 400, 410-429 (1992)
	A spatial, kinematical and dynamical analysis of Abell 400.
o	col. (9): [D80] ACO 400. [BGH92] 0254+0556 appears twice. In SIMBAD, i t has been cross-id. with [BGH92] 40, not 43.
o	Table 1, col (1): <[BGH92] HHMM+DDMMA> N=107, Table 1, col (2): <[BGH92] NN> N=99
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGH92a]
[BGH92a]	(Beers+Gebhardt+Huchra+, 1992)
*****	Avoid the usage of [BGH92a], prefer [BGH92]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGH92b]
[BGH92b]	(Burg+Giacconi+Huchra+, 1992)= (NEPX1)
Write:	<<[BGH92b] NEPX1-A>>
N:	7
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	ROSAT NEP field
in source:	NAME NEP X1
Ref:	=1992A&A...259L...9B
by	BURG R. , GIACCONI R., HUCHRA J., MacKENTY J., McLEAN B., GELLER M., HASINGER G., MARZKE R., SCHMIDT M., TRUMPER J.
	Astron. Astrophys., 259, 9-11 (1992)
	Discovery of intermediate redshift galaxy clusters in the ROSAT NEP field.
o	<NAME NEP X1>. Table 1: <[BGH92b] NEPX1-A> N=7 among (Nos A-L)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGJ2011]
[BGJ2011]	(Bauer+Grutzbauch+Jorgensen+, 2011)
Write:	<<[BGJ2011] NN>>
N:	82
Object:	G (SIMBAD class: Galaxy)
Note:	Gemini North NIRI observations of N=82 galaxies in the ClG J2235-2557 galaxy cluster.
in source:	ClG J2235-2557
Ref:	=2011MNRAS.411.2009B
by	BAUER A.E. , GRUTZBAUCH R., JORGENSEN I., VARELA J., BERGMANN M.
	Mon. Not. R. Astron. Soc., 411, 2009-2018 (2011)
	Star formation in the XMMU J2235.3-2557 galaxy cluster at z= 1.39.
o	Table 1: <[BGJ2011] NN> (Nos 1-82).
=E=	Catalogue in electronic form as <J/MNRAS/411/2009/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGK2002]
[BGK2002]	(Bresolin+Gieren+Kudritzki+, 2002)
Write:	<<[BGK2002] ANN>>
N:	19+19+19+18
Object:	Supergiant (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Spectroscopy of blue supergiant candidates in 4 fields A to D in NGC 300.
in source:	NGC 300
Ref:	=2002ApJ...567..277B
by	BRESOLIN F. , GIEREN W., KUDRITZKI R.-P., PIETRZYNSKI G., PRZYBILLA N.
	Astrophys. J., 567, 277-288 (2002)
	Spectroscopy of blue supergiants in the spiral galaxy NGC 300.
o	Table 2: <[BGK2002] ANN> (Nos A1-A19, B1-B19, C1-C19, D1-D18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGK2003]
[BGK2003]	(Barton Gillepsie+Geller+Kenyon, 2003)
Write:	<<[BGK2003] BHHMMSS.s+DDMMSS>>
N:	190
Object:	G in Pair or in Group (SIMBAD class: GinPair = Galaxy in Pair of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Spectroscopic and Photometric sample (SP sample) of galaxies in Pair or in Group.
Ref:	=2003ApJ...582..668B
by	BARTON GILLESPIE E. , GELLER M.J., KENYON S.J.
	Astrophys. J., 582, 668-688 (2003)
	Tidally triggered star formation in close pairs of galaxies. II. Constraints on burst strengths and ages.
o	Table 1: <[BGK2003] BHHMMSS.s+DDMMSS> N=190.
=E=	Catalogue in electronic form as J/ApJ/582/668
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGK2006]
[BGK2006]	(Brown+Geller+Kenyon+, 2006)= (HVS)
Write:	<<[BGK2006] HV NN>> <<[BGK2006] JHHMMSS.ss+DDMMSS.s>>
N:	22+990
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Survey of HyperVelocity Stars (HVS).
Ref:	=2006ApJ...640L..35B
by	BROWN W.R. , GELLER M.J., KENYON S.J., KURTZ M.J.
	Astrophys. J., 640, 35-38 (2006)
	A successful targeted search for hypervelocity stars.
o	Table 1: <[BGK2006] HV N> (Nos 1-5).
Ref:	=2006ApJ...647..303B
by	BROWN W.R. , GELLER M.J., KENYON S.J., KURTZ M.J.
	Astrophys. J., 647, 303-311 (2006)
	Hypervelocity stars. I. The spectroscopic survey.
o	Parag 6.2 : SDSS J172004.07+575110.8 = [BS61] 517
o	Table 1: <[BGK2006] HV N> (Nos 6-7) added. Table2, 3: <[BGK2006] JHHMMSS.ss+DDMMSS.s> N=202+44.
Ref:	=2007ApJ...660..311B
by	BROWN W.R. , GELLER M.J., KENYON S.J., KURTZ M.J., BROMLEY B.C.
	Astrophys. J., 660, 311-318 (2007)
	Hypervelocity stars. II. The bound population.
o	Table 2: <[BGK2006] JHHMMSS.ss+DDMMSS.s> N=643.
Ref:	=2007ApJ...671.1708B
by	BROWN W.R. , GELLER M.J., KENYON S.J., KURTZ M.J., BROMLEY B.C.
	Astrophys. J., 671, 1708-1716 (2007)
	Hypervelocity stars. III. The space density and ejection history of main-sequence stars from the Galactic Center.
o	Table 1: <[BGK2006] HV NN> (Nos 8-10) added. Table 2: <[BGK2006] JHHMMSS.ss+DDMMSS.s> N=381.
Ref:	=2009ApJ...690.1639B
by	BROWN W.R. , GELLER M.J., KENYON S.J.
	Astrophys. J., 690, 1639-1647 (2009)
	MMT hypervelocity star survey.
o	Table 1: <[BGK2006] HV NN> (Nos 11-16) added. Tables 1, 2: <[BGK2006] JHHMMSS.ss+DDMMSS.s> N=4+28 added.
Ref:	=2012ApJ...751...55B
by	BROWN W.R. , GELLER M.J., KENYON S.J.
	Astrophys. J., 751, 55 (2012)
	MMT hypervelocity star survey. II. Five new unbound stars.
o	Table 1: <[BGK2006] HV NN> (Nos 17-21) added.
Ref:	=2014ApJ...787...89B
by	BROWN W.R. , GELLER M.J., KENYON S.J.
	Astrophys. J., 787, 89 (2014)
	MMT hypervelocity star survey. III. The complete survey.
o	Table 1: <[BGK2006] HV NN> (Nos 22-24) added.
=E=	Catalogue in electronic form as J/ApJ/647/303
=E=	Catalogue in electronic form as J/ApJ/660/311
=E=	Catalogue in electronic form as J/ApJ/671/1708
=E=	Catalogue in electronic form as J/ApJ/751/55
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGK2007]
[BGK2007]	(Berciano Alba+Garrett+Koopmans+, 2007)
Write:	<<[BGK2007] RaN>> <<[BGK2007] Fa>>
N:	9+5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Archival VLA 1.4GHz observations of 1E 0451.6-0305. Lensed sources have the format RaNR, field sources a format Fa. see also [BCD2004].
in source:	1E 0451.6-0305 = ClG 0451-0305
Ref:	=2007A&A...462..903B
by	BERCIANO ALBA A. , GARRETT M.A., KOOPMANS L.V.E., WUCKNITZ O.
	Astron. Astrophys., 462, 903-911 (2007)
	Highly-magnified, multiply-imaged radio counterparts of the sub-mm starburst emission in the cluster-lens MS 0451.6-0305.
o	Tables: <[BGK2007] RaN> (Nos Ra1-Ra3, Rb1-Rb3, Rc1-Rc3), <[BGK2007] Fa> (Nos Fa-Fe).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGK2008]
[BGK2008]	(Barnard+Greening+Kolb, 2008)
Write:	<<[BGK2008] SNNN>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton observations of NGC 253.
in source:	NGC 253
Ref:	=2008MNRAS.388..849B
by	BARNARD R. , SHAW GREENING L., KOLB U.
	Mon. Not. R. Astron. Soc., 388, 849-862 (2008)
	A multi-coloured survey of NGC253 with XMM-Newton: testing the methods used for creating luminosity functions from low-count data.
o	Table A1: <[BGK2008] SNNN> (Nos S1-S185).
=E=	Catalogue in electronic form as J/MNRAS/388/849
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGK2009]
[BGK2009]	(Bresolin+Gieren+Kudritzki+, 2009)
Write:	<<[BGK2009] NN>>
N:	28
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	VLT FORS2 multi-object spectroscopy of N=28 HII regions in NGC 300.
in source:	NGC 300
Ref:	=2009ApJ...700..309B
by	BRESOLIN F. , GIEREN W., KUDRITZKI R.-P., PIETRZYNSKI G., URBANEJA M.A., CARRARO G.
	Astrophys. J., 700, 309-330 (2009)
	Extragalactic chemical abundances: do H II regions and young stars tell the same story? the case of the spiral galaxy NGC 300.
o	Fig. 1, Table 2: <[BGK2009] NN> (Nos 1-28).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGK2011]
[BGK2011]	(Bond+Gawiser+Koekemoer, 2011)
Write:	<<[BGK2011] PNN>>
N:	15
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST ACS and WFC3 imaging of the GOODS-S field.
in source:	NAME GOODS South Field
Ref:	=2011ApJ...729...48B
by	BOND N.A. , GAWISER E., KOEKEMOER A.M.
	Astrophys. J., 729, 48 (2011)
	Differential morphology between rest-frame optical and ultraviolet emission from 1.5 < z < 3 star-forming galaxies.
o	Table 2, Fig. 6: <[BGK2011] PNN> (Nos P1-15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGK2013]
[BGK2013]	(Beichman+Gelino+Kirkpatrick+, 2013)
Write:	<<[BGK2013] DDD.dddddddd+DD.dddddddd>>
N:	38
Object:	* (SIMBAD class: Star)
Note:	HST WFC3 observations of the field of NAME WISEP J1828+2650.
in source:	NAME WISEP J1828+2650
Ref:	=2013ApJ...764..101B
by	BEICHMAN C. , GELINO C.R., KIRKPATRICK J.D., BARMAN T.S., MARSH K.A., CUSHING M.C., WRIGHT E.L.
	Astrophys. J., 764, 101 (2013)
	The coldest brown dwarf (or free-floating planet)?: the Y dwarf WISE 1828+2650.
o	Table 3: <[BGK2013] DDD.dddddddd+DD.dddddddd> N=38.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGK87]
[BGK87]	(Bachiller+Guilloteau+Kahane, 1987)
Write:	<<[BGK87] IC 348 A>>
N:	3
Object:	NH3 Clump (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Effelsberg observations N=3 NH3 clumps in IC 348 around NAME IC 348-IR.
in source:	IC 348
Ref:	=1987A&A...173..324B
by	BACHILLER R. , GUILLOTEAU S., KAHANE C.
	Astron. Astrophys., 173, 324-336 (1987)
	Clumps in IC 348 : temperature and density profiles of dense cores.
o	Fig.2a: <[BGK87] IC 348 A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGL2004]
[BGL2004]	(Brogan+Goss+Lazendic+, 2004)
Write:	<<[BGL2004] 30 Dor OH(N)>> <<[BGL2004] N49 OH>>
N:	1+3
Object:	OH Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	ATCA observations to search for OH masers in 30 Dor nebula and LHA 120-N 49 (N49) in the LMC.
in source:	Magellanic Clouds:LMC:30 Dor Nebula = 30 Dor Nebula
in source:	Magellanic Clouds:LMC:LHA 120-N 49 = LHA 120-N 49
Ref:	=2004AJ....128..700B
by	BROGAN C.L. , GOSS W.M., LAZENDIC J.S., GREEN A.J.
	Astron. J., 128, 700-708 (2004)
	OH (1720 MHz) maser search toward the Large Magellanic Cloud.
o	<[BGL2004] 30 Dor OH(N)> (Nos 1-3), <[BGL2004] N49 OH> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGL85]
[BGL85]	(Berlin+Gol'nev+Lipovka+, 1985)
Write:	<<[BGL85] NN>>
N:	63
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1985AZh....62..229B
by	BERLIN A.B. , GOL'NEV V.Y., LIPOVKA N.M., NIZHEL'SKIJ N.A., SPANGENBERG E.E.
	Astron. Zh., 62, 229-233 (1985)
	Results of observations made at Ratan-600 with the high-sensitivity radiometer at the wavelength 7,6 cm of the region of the galaxy in the interval α=17h30m-19h30m, δ=-25.21 -22.20 (1950).
o	Table: <[BGL85] NN> (Nos 1-63)
=E=	Catalogue in electronic form as J/AZh/62/229
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BGLO
BGLO	(Blanco+Graham+Lasker+Osmer)
Write:	<<BGLO Cen A Knot A>> <<BGLO Cen A Knot AN>> <<BGLO Cen A Knot ANa>> <<BGLO Cen A Knot AN/N>> <<BGLO Cen A Knot AA>>
N:	7+11+6
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Study of optical filaments and knots in the radio-jet of NGC 5128 = Cen A. Radio, X-ray, and optical knots and overall structure of the jet are in good positional agreement. Knot A is divided into 4 sub-components (Nos A1-A4). Knot A1 is divided into 3 sub-knots (Nos A1a-A1c). A new knot is found between knots A2 and A3, named 'A2/3' by the authors. A X-ray knot is found with no distinct radio counterpart, named 'AX' by the authors. See also [KFJ2002] See also [CBF86], [HWK2003]
in source:	Cen A = NGC 5128
Ref:	=1975ApJ...198L..63B
by	BLANCO V.M. , GRAHAM J.A., LASKER B.M., OSMER P.S.
	Astrophys. J., 198, 63-64 (1975)
	Optical condensations and filaments in the northeast radio lobe of NGC 5128.
o	Figs 2,3: <BGLO Cen A Knot A> (Nos A-D).
Ref:	=1981ApJ...251...31F
by	FEIGELSON E.D. , SCHREIER E.J., DELVAILLE J.P., GIACCONI R., GRINDLAY J.E., LIGHTMAN A.P.
	Astrophys. J., 251, 31-51 (1981)
	The X-ray structure of Centaurus A.
o	Table 2, Figs: <BGLO Cen A Knot A> (Nos E-G) added.
Ref:	=1983ApJ...273..128B
by	BURNS J.O. , FEIGELSON E.D., SCHREIER E.J.
	Astrophys. J., 273, 128-153 (1983)
	The inner radio structure of Centaurus A : clues to the origin of the jet X-ray emission.
o	Fig.3, Table 2: <BGLO Cen A Knot AN> (Nos A1-A4, N1).
Ref:	=1986ApJ...300L..41C
by	CLARKE D.A. , BURNS J.O., FEIGELSON E.D.
	Astrophys. J., 300, 41-46 (1986)
	Limb brightening and filamentation in the inner radio jet of Centaurus A.
o	Knots are BGLO objects in SIMBAD, Streamers are [CBF86] SN.
o	Table 1, Fig.1: <BGLO Cen A Knot A1a> (Nos A1a-A1c), <[CBF86] SN> (Nos S1-S4).
Ref:	=1998ApJ...502..245G
by	GRAHAM J.A.
	Astrophys. J., 502, 245-252 (1998)
	Shocked gas and star formation in the Centaurus A radio galaxy.
o	Fig.2: <BGLO Cen A Knot A> (Nos X, Y, Z) added.
Ref:	=2000ApJ...531L...9K
by	KRAFT R.P. , FORMAN W., JONES C., KENTER A.T., MURRAY S.S., ALDCROFT T.L., ELVIS M.S., EVANS I.N., FABBIANO G., ISOBE T., JERIUS D., KAROVSKA M., KIM D.-W., PRESTWICH A.H., PRIMINI F.A., SCHWARTZ D.A., SCHREIER E.J., VIKHLININ A.A.
	Astrophys. J., 531, 9-12 (2000)
	A Chandra high-resolution X-ray image of Centaurus A.
o	p.12: Chandra observations, not yet registered at time of publication : CXOU (Chandra X-ray Observatory, Unregistred) acronym, not CXO.
o	Fig.3: <BGLO Cen A Knot A2/3>, <BGLO Cen A Knot AX>.
Ref:	=2003ApJ...593..169H
by	HARDCASTLE M.J. , WORRALL D.M., KRAFT R.P., FORMAN W.R., JONES C., MURRAY S.S.
	Astrophys. J., 593, 169-183 (2003)
	Radio and X-ray observations of the jet in Centaurus A.
o	The knots designated as 'S1' and 'S2' in Fig.1 and in the text are [CBF86] SL1 and [CBF86] SL2 in SIMBAD ('SL1' and 'SL2' in 1992ApJ...395..444C).
o	Fig.1: <BGLO Cen A Knot ANa> (Nos A2a, A3a, A3b, A5a, A6a, B1a) added. Fig.1: <[HWK2003] SJN> (Nos SJ1 to SJ3), <[HWK2003] SNA> (Nos S1-S2, S2A, S2B). Fig.5: <[KFJ2002] AXNA> (Nos AX1A, AX1C, SX1, SX2A, SX2B) added.
Origin	of the Acronym: L (1978ApJ...226L..79O)
Details on Acronym: [BGM2003]
[BGM2003]	(Brooks+Garay+Mardones+, 2003) (Not yet in Simbad)
Write:	<<[BGM2003] AN>>
N:	3+13
Object:	H2 Knot (SIMBAD class: PartofCloud = Part of Cloud)
Note:	VLT Infrared Spectrometer and Array Camera observations of a chain of H2 emisssion knots associated with IRAS 16547-4247 radio jet. There are 3 main concentrations of knots (Nos A-C) and several knots in each concentration.
Ref:	=2003ApJ...594L.131B
by	BROOKS K.J. , GARAY G., MARDONES D., BRONFMAN L.
	Astrophys. J., 594, 131-134 (2003)
	A parsec-scale flow associated with the IRAS 16547-4247 radio jet.
o	Fig.1, Table 1: <[BGM2003] AN> (Nos A-C, A1-A5, B1-B6, C1-C2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGM2005]
[BGM2005]	(Belanger+Goldwurm+Melia+, 2005)= ([BGM2005a])
Write:	<<[BGM2005] JHHMMSS.ss+DDMMSS.ss>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of Sgr A*: detection of two flaring sources on 2004 March 31 and 2004 August 31.
in source:	NAME Sgr A*
Ref:	=2005ApJ...635.1095B
by	BELANGER G. , GOLDWURM A., MELIA F., FERRANDO P., GROSSO N., PORQUET D., WARWICK R., YUSEF-ZADEH F.
	Astrophys. J., 635, 1095-1102 (2005)
	Repeated X-ray flaring activity in Sagittarius A.*
o	Paragr. 3.1: <[BGM2005] JHHMMSS.ss+DDMMSS.ss> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGM2005a]
[BGM2005a]	(Belanger+Goldwurm+Melia+, 2005)
*****	Avoid the usage of [BGM2005a], prefer [BGM2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGM2005b]
[BGM2005b]	(Bianchi+Guainazzi+Matt+, 2005)
Write:	<<[BGM2005b] NGC 7674 XN>> <<[BGM2005b] IRAS 13218+0552 XN>> <<[BGM2005b] NGC 1667 XN>>
N:	5+2+3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations. Brightest sources in the 3 fields: NGC 7674, IRAS 13218+0552, NGC 1667.
in source:	NGC 7674
in source:	IRAS 13218+0552
in source:	NGC 1667
Ref:	=2005A&A...442..185B
by	BIANCHI S. , GUAINAZZI M., MATT G., CHIABERGE M., IWASAWA K., FIORE F., MAIOLINO R.
	Astron. Astrophys., 442, 185-194 (2005)
	A search for changing-look AGN in the Grossan catalog.
o	Table 6: <[BGM2005b] NGC 7674 XN> (Nos X1-X5), <[BGM2005b] IRAS 13218+0552 XN> (Nos X1-X2), <[BGM2005b] NGC 1667 XN> (Nos X1-X3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGM2011]
[BGM2011]	(Bradford+Geha+Munoz+, 2011)
Write:	<<[BGM2011] CFHT NNNA>> <<[BGM2011] LRIS NNNAA>> <<[BGM2011] PAL13-SNNN>> <<[BGM2011] SERENDIP N>> <<[BGM2011] STETSON NNNNN>>
N:	298 (SIMBAD class: Star)
Note:	Keck/DEIMOS spectroscopy and CFHT/MegaCam photometry of Palomar 13.
in source:	Cl Pal 13
Ref:	=2011ApJ...743..167B
by	BRADFORD J.D. , GEHA M., MUNOZ R.R., SANTANA F.A., SIMON J.D., COTE P., STETSON P.B., KIRBY E., DJORGOVSKI S.G.
	Astrophys. J., 743, 167 (2011)
	Structure and dynamics of the globular cluster Palomar 13.
o	(Erratum) erratum vol. 778, art. 85 (2013)
o	Table 3: <[BGM2011] CFHT NNNA>, <[BGM2011] LRIS NNNAA>, <[BGM2011] PAL13-SNNN>, <[BGM2011] SERENDIP N>, <[BGM2011] STETSON NNNNN> N=298.
=E=	Catalogue in electronic form as <J/ApJ/743/167/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGM2011b]
[BGM2011b]	(Bouy+Girard+Martin+, 2011)
Write:	<<[BGM2011b] JHHMMSS.ss+DDMMSS.s>>
N:	8 (SIMBAD class: Star)
Note:	VLT NACO observations of the field of UGPS J072227.51-054031.2.
Ref:	=2011A&A...526A..55B
by	BOUY H. , GIRARD J.H.V., MARTIN E.L., HUELAMO N., LUCAS P.W.
	Astron. Astrophys., 526A, 55-55 (2011)
	Adaptive optics observations of the T10 ultracool dwarf UGPS J072227.51-054031.2.
o	Table 1, Figure 1 : <[BGM2011b] JHHMMSS.ss+DDMMSS.s> N=8
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGM2013]
[BGM2013]	(Barnard+Garcia+Murray, 2013)
Write:	<<[BGM2013] BHC NN>>
N:	35
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of N=35 black hole candidates (BHC) in the central region of M31.
in source:	M 31 = NGC 224
Ref:	=2013ApJ...770..148B
by	BARNARD R. , GARCIA M.R., MURRAY S.S.
	Astrophys. J., 770, 148 (2013)
	Chandra identification of 26 new black hole candidates in the central region of M31.
o	Fig. 2, Tables 1-3: <[BGM2013] BHC NN> (Nos 1-35).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGM2017]
[BGM2017]	(Balmaverde+Gilli+Mignoli+, 2017)= ([BGM2017a])
Write:	<<[BGM2017] J1030 NNNNN>> <<[BGM2017] J1148 NNNNN>> <<[BGM2017] J1048 NNNNN>> <<[BGM2017] J1411 NNNNN>>
N:	69+18
Object:	Poss. LBG (SIMBAD class: Galaxy_Candidate = Galaxy Candidate)
Note:	LCFHT WIRCam and BT LBC deep photometric observations of N=69+18 Lyman break galaxy candidates in the field of four high-redshift (z∼6) QSOs.
in source:	QSO B1027+0540
in source:	QSO J1148+5251
in source:	QSO J1048+4637
in source:	QSO J1411+1217
Ref:	=2017A&A...606A..23B
by	BALMAVERDE B. , GILLI R., MIGNOLI M., BOLZONELLA M., BRUSA M., CAPPELLUTI N., COMASTRI A., SANI E., VANZELLA E., VIGNALI C., VITO F., ZAMORANI G.
	Astron. Astrophys., 606A, 23-23 (2017)
	Primordial environment of supermassive black holes. II. Deep Y- and J-band images around the z~ 6.3 quasar SDSS J1030+0524.
o	Tables 2: <[BGM2017] J1030 NNNNN> N=18 among (Nos 2335 to 30511) added.
Ref:	=2014A&A...568A...1M
by	MORSELLI L. , MIGNOLI M., GILLI R., VIGNALI C., COMASTRI A., SANI E., CAPPELLUTI N., ZAMORANI G., BRUSA M., GALLOZZI S., VANZELLA E.
	Astron. Astrophys., 568A, 1-1 (2014)
	Primordial environment of super massive black holes: large-scale galaxy overdensities around z ~ 6 quasars with LBT.
o	Tables 2-3: <[BGM2017] J1030 NNNNN> N=14+10 among (Nos 2140 to 28941), <[BGM2017] J1148 NNNNN> N=8+3 among (Nos 1556 to 18368), <[BGM2017] J1048 NNNNN> N=6+9 among (Nos 2968 to 22521), <[BGM2017] J1411 NNNNN> N=11+8 among (Nos 564 to 25638).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGM2017b]
[BGM2017b]	(Balogh+Gilbank+Muzzin+, 2021)
Write:	<<[BGM2017b] COSMOS-NNN>>
N:	4
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	N=4 X-ray selected galaxy groups in the COSMOS field. Use of Gemini GMOS spectroscopy.
in source:	NAME COSMOS Field
Ref:	=2017MNRAS.470.4168B
by	BALOGH M.L. , GILBANK D.G., MUZZIN A., RUDNICK G., COOPER M.C., LIDMAN C., BIVIANO A., DEMARCO R., McGEE S.L., NANTAIS J.B., NOBLE A., OLD L., WILSON G., YEE H.K.C., BELLHOUSE C., CERULO P., CHAN J., PINTOS-CASTRO I., SIMPSON R., VAN DER BURG R.F.J., ZARITSKY D., ZIPARO F., ALONSO M.V., BOWER R.G., DE LUCIA G., FINOGUENOV A., LAMBAS D.G., MURIEL H., PARKER L.C., RETTURA A., VALOTTO C., WETZEL A.
	Mon. Not. R. Astron. Soc., 470, 4168-4185 (2017)
	Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: survey description.
o	Table 1: <[BGM2017b] COSMOS-NNN> N=4 among (Nos 28-221).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGM2021]
[BGM2021]	(Brand+Giannetti+Massi+, 2021)
Write:	<<[BGM2021] NNN>>
N:	686
Object:	Dense Core (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	JCMT SCUBA-2 (450 and 850µm) and HARP (CO(3-2)) observations of N=686 dense cores in NGC 6357. Use of Herschel Hi-GAL data at 70 and 160µm.
in source:	NGC 6357
Ref:	=2021A&A...647A.154B
by	BRAND J. , GIANNETTI A., MASSI F., WOUTERLOOT J.G.A., VERDIRAME C.
	Astron. Astrophys., 647A, 154-154 (2021)
	A possible far-ultraviolet flux-dependent core mass function in NGC 6357.
o	Table 2: <[BGM2021] NNN> (Nos 1-686).
=E=	Catalogue in electronic form as <J/A+A/647/A154/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [BGN2005]
[BGN2005]	(Brooks+Garay+Nielbock+, 2005)
Write:	<<[BGN2005] JHHMMSS.s+DDMMSS>>
N:	11
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Observations of the SIMBA bolometer at SEST, to measure the 1.2mm continuum emission toward the Keyhole nebula. 11 clumps are detected, corresponding to bright-rimmed molecular globules.
in source:	NAME Keyhole Nebula
Ref:	=2005ApJ...634..436B
by	BROOKS K.J. , GARAY G., NIELBOCK M., SMITH N., COX P.
	Astrophys. J., 634, 436-441 (2005)
	SIMBA observations of the Keyhole nebula.
o	Table 1: <[BGN2005] JHHMMSS.s+DDMMSS> N=11.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BGP
BGP	(Bucknell+Godwin+Peach)
Write:	<<BGP ACO NNNN NNN>>
N:	1000
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Table A1: N=233 G in ACO 426 Table A3: N=144 G in ACO 1553 Table A4: N=156 G in ACO 2065 Table A5: N=170 G in ACO 2147 Table A6: N=154 G in ACO 2151 Table A8: N=143 G in ACO 2670 Table A2: G in ACO 1377, numbering following and extending [B28] Table A7: G in ACO 2199, numbering following and extending [RS72] See also [AP74], [AGP75], BGP, GP, [GP82]
in source:	ACO 426
in source:	ACO 1553
in source:	ACO 2065
in source:	ACO 2147
in source:	ACO 2151
in source:	ACO 2670
Ref:	=1979MNRAS.188..579B
by	BUCKNELL M.J. , GODWIN J.G., PEACH J.V.
	Mon. Not. R. Astron. Soc., 188, 579-593 (1979)
	Studies of rich clusters of galaxies- V. Photometry and luminosity functions for eight clusters.
o	Table A1: <BGP ACO 426 NNN> (Nos 1-233). Table A3: <BGP ACO 1553 NNN> (Nos 1-144). Table A4: <BGP ACO 2065 NNN> (Nos 1-156). Table A5: <BGP ACO 2147 NNN> (Nos 1-170). Table A6: <BGP ACO 2151 NNN> (Nos 1-154). Table A8: <BGP ACO 2670 NNN> (Nos 1-143). Table A2: <[B28] NNN> (Nos 60-114) added. Table A7: <[RS72] NNN> (Nos 201-272) added.
Origin	of the Acronym: L (1997A&AS..126...67A)
Details on Acronym: [BGP2012]
[BGP2012]	(Bontempi+Giroletti+Panessa+, 2012)
Write:	<<[BGP2012] NGC NNNN C>> <<[BGP2012] NGC NNNN WN>>
N:	4+5
Object:	(Rad) + Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	1.5 and 5GHz European VLBI observations of the central region of Seyfert galaxies.
in source:	NGC 3227
in source:	NGC 3982
in source:	NGC 4138
in source:	NGC 4477
Ref:	=2012MNRAS.426..588B
by	BONTEMPI P. , GIROLETTI M., PANESSA F., ORIENTI M., DOI A.
	Mon. Not. R. Astron. Soc., 426, 588-594 (2012)
	Physical properties of the nuclear region in Seyfert galaxies derived from observations with the European VLBI Network.
o	Figs 1-3, Table 4: <[BGP2012] NGC NNNN C> N=4, <[BGP2012] NGC NNNN WN> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGP2014]
[BGP2014]	(Barnard+Garcia+Primini+, 2014)
Write:	<<[BGP2014] NNN>>
N:	528
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of N=528 X-ray sources in the central 20' of M31.
in source:	M 31 = NGC 224
Ref:	=2014ApJ...780...83B
by	BARNARD R. , GARCIA M.R., PRIMINI F., LI Z., BAGANOFF F.K., MURRAY S.S.
	Astrophys. J., 780, 83 (2014)
	Around 200 new X-ray binary IDs from 13 yr of Chandra observations of the M31 center.
o	Table 1: <[BGP2014] NNN> (Nos 1-528).
=E=	Catalogue in electronic form as <J/ApJ/780/83/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGP87]
[BGP87]	(Braun+Gull+Perley, 1987) (Not yet in Simbad)
Write:	<<[BGP87] A>>
N:	11
Object:	Feature (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLA observations of Cas A.
in source:	NAME Cas A
Ref:	=1987Natur.327..395B
by	BRAUN R. , GULL S.F., PERLEY R.A.
	Nature, 327, 395-399 (1987)
	Physical process which shapes Cassiopeia A.
o	Table 1: <[BGP87] A> (Nos A-K).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BGPS
BGPS	(Bolocam Galactic Plane Survey)
Write:	<<BGPS GLLL.lll+BB.bbb>>
N:	8358
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	CSO Bolocam observations at 268GHz (1.1mm) of the millimeter dust continuum emission from the northern Galactic plane.
Ref:	=2010ApJS..188..123R
by	ROSOLOWSKY E. , DUNHAM M.K., GINSBURG A., BRADLEY E.T., AGUIRRE J., BALLY J., BATTERSBY C., CYGANOWSKI C., DOWELL D., DROSBACK M., EVANS N.J., GLENN J., HARVEY P., STRINGFELLOW G.S., WALAWENDER J., WILLIAMS J.P.
	Astrophys. J., Suppl. Ser., 188, 123-138 (2010)
	The Bolocam Galactic Plane Survey. II. Catalog of the image data.
o	Table 1: <BGPS GLLL.lll+BB.bbb> N=8358.
=E=	Catalogue in electronic form as <J/ApJS/188/123/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BGPSv2
BGPSv2	(Bolocam Galactic Plane Survey v2)
Write:	<<BGPSv2 GLLL.lll+BB.bbb>> <<BGPSv2 NNNN>>
N:	8594+8594
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	This is a re-reduction and expansion of the Bolocam Galactic Plane Survey (BGPS). The BGPS is a 1.1 mm survey of dust emission in the Northern galactic plane, covering longitudes –10deg<l<90deg and latitudes \|b\|<0.5deg with a typical 1σ rms sensitivity of 30-100mJy in a ∼33" beam. Version 2 of the survey includes an additional ∼20deg² of coverage in the third and fourth quadrants and ∼2deg² in the first quadrant. The BGPS V2 catalog (N=8594 objects) is available at http://irsa.ipac.caltech.edu/data/BOLOCAM_GPS
Ref:	=2013ApJS..208...14G
by	GINSBURG A. , GLENN J., ROSOLOWSKY E., ELLSWORTH-BOWERS T.P., BATTERSBY C., DUNHAM M., MERELLO M., SHIRLEY Y., BALLY J., EVANS II N.J., STRINGFELLOW G., AGUIRRE J.
	Astrophys. J., Suppl. Ser., 208, 14 (2013)
	The Bolocam Galactic Plane Survey. IX. Data release 2 and outer galaxy extension.
o	<BGPSv2 NNNN> (Nos 1-8594) = <BGPSv2 GLLL.lll+BB.bbb> N=8594.
=E=	Catalogue in electronic form as <J/ApJS/208/14/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BGPSv2
BGPSv2	(Bolocam Galactic Plane Survey v2)
*****	Avoid the usage of BGPSv2, prefer [ERG2015]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BGR2000]
[BGR2000]	(Borissova+Georgiev+Rosado+, 2000)= (Br)
Write:	<<[BGR2000] Br N>>
N:	6
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=6 Brackett gamma knots or emission features in IC 10.
in source:	IC 10
Ref:	=2000A&A...363..130B
by	BORISSOVA J. , GEORGIEV L., ROSADO M., KURTEV R., BULLEJOS A., VALDEZ-GUTIERREZ M.
	Astron. Astrophys., 363, 130-140 (2000)
	Infrared photometry of the Local Group dwarf irregular galaxy IC 10.
o	Table 1: <[BGR2000] Br N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGR2011]
[BGR2011]	(Baran+Gilker+Reed+, 2011)
Write:	<<[BGR2011] J08069+1527>>
N:	1
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	KPNO 2.1-m telescope photometry, and Baker Observatory and La Palma Mercator telescope follow-up observations.
Ref:	=2011MNRAS.413.2838B
by	BARAN A.S. , GILKER J.T., REED M.D., OSTENSEN R.H., TELTING J.H., SMOLDERS K., HICKS L., OREIRO R.
	Mon. Not. R. Astron. Soc., 413, 2838-2844 (2011)
	J08069+1527: a newly discovered high-amplitude, hybrid subdwarf B pulsator.
o	<[BGR2011] J08069+1527> N=1.
o	The sdB star J08069+1527 is 2MASS J08065668+1527200 in Simbad.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGS2002]
[BGS2002]	(Butler+Golden+Shearer, 2002)
Write:	<<[BGS2002] Star a>> <<[BGS2002] NNHST>>
N:	2+14
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of the field around PSR 1951+32. see also [BS85].
Ref:	=2002A&A...395..845B
by	BUTLER R.F. , GOLDEN A., SHEARER A.
	Astron. Astrophys., 395, 845-851 (2002)
	Detection of new optical counterpart candidates to PSR B1951+32 with HST/WFPC2.
o	Fig.1: <[BGS2002] Star a> (Nos w, y). Table 3: <[BGS2002] NNHST> (Nos 1HST to 14HST).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGS2006]
[BGS2006]	(Boschin+Girardi+Spolaor+, 2006)
Write:	<<[BGS2006] NNN>>
N:	102
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Use of archival NTT EMMI observations. Detailed dynamical analysis of the rich galaxy cluster ACO 2744.
in source:	ACO 2744 = ACCG 118
Ref:	=2006A&A...449..461B
by	BOSCHIN W. , GIRARDI M., SPOLAOR M., BARRENA R.
	Astron. Astrophys., 449, 461-474 (2006)
	Internal dynamics of the radio halo cluster Abell 2744.
o	Table 1: <[BGS2006] NNN> (Nos 1-102).
=E=	Catalogue in electronic form as J/A+A/449/461
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGS2006a]
[BGS2006a]	(Boschin+Girardi+Spolaor+, 2006)
*****	Avoid the usage of [BGS2006a], prefer [BGS2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGS2006b]
[BGS2006b]	(Blair+Ghavamian+Sankrit+, 2006)
Write:	<<[BGS2006b] JHHMM+DDd>> <<[BGS2006b] JHHMM+DDda>> <<[BGS2006b] JHHMM.m+DDMM>>
N:	24
Object:	SNR (SIMBAD class: SNRemnant = SuperNova Remnant)
Stat:	is completely incorporated in Simbad
Note:	FUSE observations of SNRs in the Magellanic Clouds.
in source:	Magellanic Clouds:LMC = LMC
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2006ApJS..165..480B
by	BLAIR W.P. , GHAVAMIAN P., SANKRIT R., DANFORTH C.W.
	Astrophys. J., Suppl. Ser., 165, 480-511 (2006)
	Far ultraviolet spectroscopic explorer survey of Magellanic cloud supernova remnants.
o	Table 2: Some of the SNR are SNR BHHMM+DD.d and not [BGS2006b], there is some confusion between 1950 and 2000 coordinates.
o	Table 2: <[BGS2006b] JHHMM+DDd>, <[BGS2006b] JHHMM+DDda>, <[BGS2006b] JHHMM.m+DDMM>, N=24.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGS2017]
[BGS2017]	(Bianchi+Giovanardi+Smith+, 2017)
Write:	<<[BGS2017] NN>>
N:	22
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Herschel SPIRE observations of N=22 diffuse excess regions at 250µm, as part of the Herschel Virgo Cluster Survey (HeViCS).
in source:	NAME Virgo Cluster
Ref:	=2017A&A...597A.130B
by	BIANCHI S. , GIOVANARDI C., SMITH M.W.L., FRITZ J., DAVIES J.I., HAYNES M.P., GIOVANELLI R., BAES M., BOCCHIO M., BOISSIER S., BOQUIEN M., BOSELLI A., CASASOLA V., CLARK C.J.R., DE LOOZE I., DI SEREGO ALIGHIERI S., GROSSI M., JONES A.P., HUGHES T.M., HUNT L.K., MADDEN S., MAGRINI L., PAPPALARDO C., YSARD N., ZIBETTI S.
	Astron. Astrophys., 597A, 130-130 (2017)
	The Herschel Virgo Cluster Survey. XX. Dust and gas in the foreground Galactic cirrus.
o	Table 3: <[BGS2017] NN> (Nos 1-22).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGS2021]
[BGS2021]	(Beuther+Gieser+Suri+, 2021)
Write:	<<[BGS2021] ISOSSHHMMm NN>>
N:	29
Object:	Core (SIMBAD class: denseCore = Dense Core)
Note:	IRAM 30m and NOEMA observations of N=15+14 cores in the two young high-mass star-forming regions ISOSS J22478+6357 and ISOSS J23053+5953.
in source:	ISOSS J22478+6357
in source:	ISOSS J23053+5953
Ref:	=2021A&A...649A.113B
by	BEUTHER H. , GIESER C., SURI S., LINZ H., KLAASSEN P., SEMENOV D., WINTERS J.M., HENNING T., SOLER J.D., URQUHART J.S., SYED J., FENG S., MOLLER T., BELTRAN M.T., SANCHEZ-MONGE A., LONGMORE S.N., PETERS T., BALLESTEROS-PAREDES J., SCHILKE P., MOSCADELLI L., PALAU A., CESARONI R., LUMSDEN S., PUDRITZ R., WYROWSKI F., KUIPER R., AHMADI A.
	Astron. Astrophys., 649A, 113 (2021)
	Fragmentation and kinematics in high-mass star formation. CORE-extension targeting two very young high-mass star-forming regions.
o	Fig. 3, Table 2: <[BGS2021] ISOSSHHMMm NN> N=15+14.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGT2011]
[BGT2011]	(Banfield+George+Taylor+, 2011)= (DRAO)
Write:	<<[BGT2011] DRAO JHHMMSS.ss+DDMMSS.ss>>
N:	16+18
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	DRAO synthesis telescope 1.4 GHz observations of the ELAIS N1 field. See also [GTS2010].
Ref:	=2011ApJ...733...69B
by	BANFIELD J.K. , GEORGE S.J., TAYLOR A.R., STIL J.M., KOTHES R., SCOTT D.
	Astrophys. J., 733, 69 (2011)
	Polarized radio sources: a study of luminosity, redshift, and infrared colors.
o	Tables 5-6: <[BGT2011] DRAO JHHMMSS.ss+DDMMSS.ss> N=16+18.
=E=	Catalogue in electronic form as J/ApJ/733/69
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGU2000]
[BGU2000]	(Brinkmann+Gliozzi+Urry+, 2001)
Write:	<<[BGU2000] JHHMMSS+DDMMSS>>
N:	1
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT HRI observation of the field of PKS 2155-304. N=1 other bright source: 'J215817-300016'.
Ref:	=2000A&A...362..105B
by	BRINKMANN W. , GLIOZZI M., URRY C.M., MARASCHI L., SAMBRUNA R.
	Astron. Astrophys., 362, 105-112 (2000)
	The soft X-Ray variability of PKS 2155-304.
o	Text: <[BGU2000] JHHMMSS+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BGV2006]
[BGV2006]	(Barkhouse+Green+Vikhlinin+, 2006)
Write:	<<[BGV2006] NNN>>
N:	102
Object:	Poss. ClG (SIMBAD class: ClG_Candidate = Cluster of Galaxies Candidate)
Note:	Survey of serendipitous extended X-ray sources (see CXOMP) and optical cluster candidates from the Chandra Multiwavelength Project (ChaMP).
Ref:	=2006ApJ...645..955B
by	BARKHOUSE W.A. , GREEN P.J., VIKHLININ A., KIM D.-W., PERLEY D., CAMERON R., SILVERMAN J., MOSSMAN A., BURENIN R., JANNUZI B.T., KIM M., SMITH M.G., SMITH R.C., TANANBAUM H., WILKES B.J.
	Astrophys. J., 645, 955-976 (2006)
	ChaMP serendipitous galaxy cluster survey.
o	Table 5 : SDSS CE J016.528793+00.817471 not identified
o	Table 4: <[BGV2006] NNN> (Nos 1-102).
=E=	Catalogue in electronic form as J/ApJ/645/955
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BH
BH	(Barmby+Huchra) (Not yet in Simbad)
*****	Avoid the usage of BH, prefer [BH2001b]
Details on Acronym: BH
BH	(Boeshaar+Hodge)
Write:	<<BH NNN>>
N:	223
Object:	HII (SIMBAD class: HIIReg = HII Region)
in source:	NGC 3631
Ref:	=1977ApJ...213..361B
by	BOESHAAR G.O. , HODGE P.W.
	Astrophys. J., 213, 361-367 (1977)
	H II regions and the spiral structure of NGC 3631.
o	Table 1: <BH NNN> (Nos 1-223)
Origin	of the Acronym: L (1988ApJ...334..144K)
Details on Acronym: BH
BH	(Bhatia+Hatzidimitriou)
*****	Avoid the usage of BH, prefer [BH88]
Origin	of the Acronym: L (1999AJ....117..238B)
Details on Acronym: BH
BH	(B and H different techniques)
*****	Avoid the usage of BH, prefer [BMA2003]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BH
BH	(van den Bergh+Hagen)
*****	Avoid the usage of BH, prefer VDBH
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BH2001]
[BH2001]	(Borkowski+Harrington, 2001)= ([BH2001a]) (Not yet in Simbad)
Write:	<<[BH2001] A>> <<[BH2001] A'>>
N:	3+3
Object:	Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Knots in the PN 'Hen 3-1475'.
in source:	Hen 3-1475
Ref:	=2001ApJ...550..778B
by	BORKOWSKI K.J. , HARRINGTON J.P.
	Astrophys. J., 550, 778-784 (2001)
	Kinematics of 1200 kilometer per second jets in He 3-1475.
o	Fig.1: <[BH2001] A> (Nos O, M, I), <[BH2001] A'> (Nos O', M', I').
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BH2001a]
[BH2001a]	(Borkowski+Harrington, 2001) (Not yet in Simbad)
*****	Avoid the usage of [BH2001a], prefer [BH2001]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BH2001b]
[BH2001b]	(Barmby+Huchra, 2001)= (BH)
Write:	<<[BH2001b] NN>>
N:	32
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	N=32 globular clusters in M31. See also M31GC.
in source:	M 31 = NGC 224
Ref:	=2001AJ....122.2458B
by	BARMBY P. , HUCHRA J.P.
	Astron. J., 122, 2458-2468 (2001)
	M 31 globular clusters in the Hubble Space Telescope archive. I. Cluster detection and completeness.
o	Tables 2, 3, 4: objects NNN-NNN, NNNA-NNN, NNN-ANNN, NNN-AANN, are [BHB2000] in SIMBAD, except for objects 000-MNNN which are [MKK98] M 31 NNN.
o	Table 3: <M31GC JHHMMSS+DDMMSS> N=32 = <[BH2001b] NN> (Nos 1-32), <M31OC JHHMMSS+DDMMSS> N=20.
Details on Acronym: [BH2018]
[BH2018]	(Baumgardt+Hilker, 2018)
Write:	<<[BH2018] JDDD.dddddd+DD.dddddd>>
N:	11522
Object:	* (SIMBAD class: Star)
Note:	N=11522 stars in the field of 54 Galactic globular clusters. Use of archival VLT and Keck spectroscopic data.
Ref:	=2018MNRAS.478.1520B
by	BAUMGARDT H. , HILKER M.
	Mon. Not. R. Astron. Soc., 478, 1520-1557 (2018)
	A catalogue of masses, structural parameters, and velocity dispersion profiles of 112 Milky Way globular clusters.
o	Tables D1-D53: <[BH2018] JDDD.dddddd+DD.dddddd> N=11522.
=E=	Catalogue in electronic form as <J/MNRAS/478/1520/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BH39]
[BH39]	(Baade+Hubble, 1939)
Write:	<<[BH39] A>> <<[BH39] NN>>
N:	2+8
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	N=2 exceptionally bright variable stars (Nos A-B), in Sculptor. N=8 of the 40 faint variable stars in Sculptor.
in source:	NAME Scl Dwarf Galaxy
Ref:	=1939PASP...51...40B
by	BAADE W. , HUBBLE E.
	Publ. Astron. Soc. Pac., 51, 40-44 (1939)
	The new stellar systems in Sculptor and Fornax.
o	Plate V: <[BH39] A> (Nos A-B), <[BH39] NN> N=8 among 40.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BH88]
[BH88]	(Bhatia+Hatzidimitriou, 1988)= (BH)
Write:	<<[BH88] HHMMSS+DDMMSS>>
N:	69
Object:	Cluster pair (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	Identification of 69 double clusters in the LMC. 39 have previously been recorded as single cluster.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1988MNRAS.230..215B
by	BHATIA R.K. , HATZIDIMITRIOU D.
	Mon. Not. R. Astron. Soc., 230, 215-221 (1988)
	Binary star clusters in the Large Magellanic Cloud.
o	Table 1: <[BH88] HHMMSS+DDMMSS> N=69.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BH95]
[BH95]	(Baan+Haschick, 1995)
Write:	<<[BH95] A>>
N:	5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
in source:	IC 4553 = APG 220
Ref:	=1995ApJ...454..745B
by	BAAN W.A. , HASCHICK A.D.
	Astrophys. J., 454, 745-748 (1995)
	Nuclear antics of IC 4553 (Arp 220).
o	Fig.4: 'OP N' = '[SDC94] N', 'OH I' 'OH IIa' 'OH IIb' = '[DNB89] OH I', 'IIa', IIb'
o	Fig.2: <[BH95] A> (Nos A-E)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BH98]
[BH98]	(Barmby+Huchra, 1988)
Write:	<<[BH98] HHMMm+DDMMW>> <<[BH98] HHMM+DDMMA>> <<[BH98] AHHMM+DDMMA>>
N:	360
Object:	G in Supercluster (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
in source:	NAME Hercules Supercluster
Ref:	=1998AJ....115....6B
by	BARMBY P. , HUCHRA J.P.
	Astron. J., 115, 6-25 (1998)
	Kinematics of the Hercules supercluster.
o	(Erratum) Erratum vol. 116, p. 1508
o	Table 1: <[BH98] HHMMm+DDMMW>, <[BH98] HHMM+DDMMA>, <[BH9] AHHMM+DDMM> N=360.
=E=	Catalogue in electronic form as J/AJ/115/6
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BHA
BHA	(Bailey+Hough+Axon)= (B)
Write:	<<BHA NNW>>
N:	35+2
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
in source:	NAME Gal Center
Ref:	=1984MNRAS.208..661B
by	BAILEY J. , HOUGH J.H., AXON D.J.
	Mon. Not. R. Astron. Soc., 208, 661-671 (1984)
	Imaging and polarimetry of the galactic centre in the near-infrared.
o	Table 1: <BHA NN> (Nos 1-35)
Ref:	=1996Natur.383..415E
by	ECKART A. , GENZEL R.
	Nature, 383, 415-417 (1996)
	Observations of stellar proper motions near the Galactic Centre.
o	Table 1: only GCIRS and BHA sources are in SIMBAD.
o	Table 1: <GCIRS NNWWN> (Nos 16SE1, 16SE2, 29N, 29S, 33E, 33W, 34W) are new. <BHA NW> (Nos 4E, 4W)
Origin	of the Acronym: L (1996Natur.383..415E)
Details on Acronym: [BHA2010]
[BHA2010]	(Brisbin+Harwit+Altieri+, 2010)
Write:	<<[BHA2010] LN A>> <<[BHA2010] GOODS A>> <<[BHA2010] GOODS a>> <<[BHA2010] LN a>>
N:	9+12+4+7
Object:	G (SIMBAD class: Galaxy)
Note:	Use of Herschel SPIRE and Spitzer 24µm data.
in source:	NAME GOODS North Field
in source:	NAME Lockman Hole North
Ref:	=2010MNRAS.409...66B
by	BRISBIN D. , HARWIT M., ALTIERI B., AMBLARD A., ARUMUGAM V., AUSSEL H., BABBEDGE T., BLAIN A., BOCK J., BOSELLI A., BUAT V., CASTRO-RODRIGUEZ N., CAVA A., CHANIAL P., CLEMENTS D.L., CONLEY A., CONVERSI L., COORAY A., DOWELL C.D., DWEK E., EALES S., ELBAZ D., FOX M., FRANCESCHINI A., GEAR W., GLENN J., GRIFFIN M., HALPERN M., HATZIMINAOGLOU E., IBAR E., ISAAK K., IVISON R.J., LAGACHE G., LEVENSON L., LONSDALE C.J., LU N., MADDEN S., MAFFEI B., MAINETTI G., MARCHETTI L., MORRISON G.E., NGUYEN H.T., O'HALLORAN B., OLIVER S.J., OMONT A., OWEN F.N., PANNELLA M., PANUZZO P., PAPAGEORGIOU A., PEARSON C.P., PEREZ-FOURNON I., POHLEN M., RIZZO D., ROSEBOOM I.G., ROWAN-ROBINSON M., SANCHEZ PORTAL M., SCHULZ B., SEYMOUR N., SHUPE D.L., SMITH A.J., STEVENS J.A., STRAZZULLO V., SYMEONIDIS M., TRICHAS M., TUGWELL K.E., VACCARI M., VALTCHANOV I., VIGROUX L., WANG L., WARD R., WRIGHT G., XU C.K., ZEMCOV M.
	Mon. Not. R. Astron. Soc., 409, 66-74 (2010)
	The deep SPIRE HerMES survey: spectral energy distributions and their astrophysical indications at high redshift.
o	Table 2, Fig. 2: <[BHA2010] LN A> (Nos A-I). Table 3, Fig. 3: <[BHA2010] GOODS A> (Nos A-L). Table 4, Fig. 5: <[BHA2010] GOODS a> (Nos a-d), <[BHA2010] LN a> (Nos e-k).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHA97]
[BHA97]	(Blaes+Hurt+Antonucci+, 1997) (Not yet in Simbad)
Write:	<<[BHA97] NN>> <<[BHA97] NN'>> <<[BHA97] A>> <<[BHA97] A'>>
N:	19+2+2+1
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT PSPC observations
Ref:	=1997ApJ...479..868B
by	BLAES O. , HURT T., ANTONUCCI R., HURLEY K., SMETTE A.
	Astrophys. J., 479, 868-874 (1997)
	Infrared observations of the possible X-ray counterpart to the 1992 may 1 γ-ray burst.
o	Table 1, Fig. 1: <[BHA97] NN> (Nos 1-19), <[BHA97] NN'> (Nos 3', 10'), <[BHA97] A> (Nos B-C), <[BHA97] A'> (No. C')
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BHB
BHB	(Blue Horizontal Branch)
*****	Avoid the usage of BHB, prefer [AG92]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BHB2000]
[BHB2000]	(Barmby+Huchra+Brodie+, 2000)
Write:	<<[BHB2000] NNN-NNN>> <<[BHB2000] NNNA-NNN>> <<[BHB2000] NNN-ANNN>> <<[BHB2000] NNN-AANN>>
N:	383
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	Catalog of photometric data for M 31 globular clusters. The catalog contains 435 GCl, 383 having formats similar to the one used in HBK. Format 'NNN-NNN' combination of Bol NNN and SKHB NNN. Format 'NNNA-NNN' combination of Bol DNNN and SKHB NNN. Format 'NNN-ANNN' combination of Bol NNN and if DNNN: [CCS85] NNN if HNNN or BNNN: [V62] NNN. Format 'NNN-AANN' combination of Bol DNNN and NBol NN.
in source:	M 31 = NGC 224
Ref:	=2000AJ....119..727B
by	BARMBY P. , HUCHRA J.P., BRODIE J.P., FORBES D.A., SCHROEDER L.L., GRILLMAIR C.J.
	Astron. J., 119, 727-747 (2000)
	M31 globular clusters: colors and metallicities.
o	T.1: Object 'EX 8' not identified.
o	Table 1: <[BHB2000] NNN-NNN>, <[BHB2000] NNNA-NNN>, <[BHB2000] NNN-ANNN>, <[BHB2000] NNN-AANN>, N=383.
=E=	Catalogue in electronic form as J/AJ/119/727
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHB2001]
[BHB2001]	(Baker+Hunstead+Bremer+, 2001) (Not yet in Simbad)
Write:	<<[BHB2001] +xx+yy>>
N:	33
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	N=33 IR sources in the field of the QSO MRC 0450-221. In the format '+xx+yy' are coordinates in arcsec. relative to the quasar position.
in source:	MRC 0450-221
Ref:	=2001AJ....121.1821B
by	BAKER J.C. , HUNSTEAD R.W., BREMER M.N., BLAND-HAWTHORN J., ATHREYA R.M., BARR J.
	Astron. J., 121, 1821-1839 (2001)
	Tunable-filter imaging of quasar fields at z~1. I. A cluster around MRC B0450-221.
o	Table 1: <[BHB2001] +xx+yy> N=33.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHB2007]
[BHB2007]	(Brooke+Huard+Bourke+, 2007)
Write:	<<[BHB2007] NNWW>>
N:	20+5
Object:	Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Stat:	is completely incorporated in Simbad
Note:	Spitzer c2d survey of the dark cloud Barn 59: search for YSO candidates. 2010ApJ...722..971C: WW added in format following IRTF SpeX observations.
in source:	Barnard 59
Ref:	=2007ApJ...655..364B
by	BROOKE T.Y. , HUARD T.L., BOURKE T.L., BOOGERT A.C.A., ALLEN L.E., BLAKE G.A., EVANS II N.J., HARVEY P.M., KOERNER D.W., MUNDY L.G., MYERS P.C., PADGETT D.L., SARGENT A.I., STAPELFELDT K.R., VAN DISHOECK E.F., CHAPMAN N., CIEZA L., DUNHAM M.M., LAI S.-P., PORRAS A., SPIESMAN W., TEUBEN P.J., YOUNG C.H., WAHHAJ Z., LEE C.W.
	Astrophys. J., 655, 364-374 (2007)
	The Spitzer c2d survey of nearby dense cores. IV. Revealing the embedded cluster in B 59.
o	Table 1: <[BHB2007] NN> (Nos 1-20).
Ref:	=2010ApJ...722..971C
by	COVEY K.R. , LADA C.J., ROMAN-ZUNIGA C., MUENCH A.A., FORBRICH J., ASCENSO J.
	Astrophys. J., 722, 971-988 (2010)
	The age, stellar content, and star formation timescale of the B59 dense core.
o	Table 2: [BHB2007] 18SW, [CLR2010] 2 and [CLR2010] 2NE are not in SIMBAD (no coordinates).
o	Fig. 1, Table 2: <[CLR2010] NWW> (Nos 1-2, 2NE-2SW, 3-9). Fig. 2, Table 1: <[BHB2007] NNWW> (Nos 8NW-8SE, 13NW, 18NE-18SW).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHB98]
[BHB98]	(Buchalter+Helfand+Becker+, 1998)
Write:	<<[BHB98] JHHMMSS.s+DDMMSS>>
N:	103
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	The authors used VLA FIRST survey to find 103 double-lobed QSO.
Ref:	=1998ApJ...494..503B
by	BUCHALTER A. , HELFAND D.J., BECKER R.H., WHITE R.L.
	Astrophys. J., 494, 503-522 (1998)
	Constraining {OMEGA}_{0} with the angular size-redshift relation of double-lobed quasars in the FIRST survey.
o	Table 1: <[BHB98] JHHMMSS.s+DDMMSS> N=103.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHC2009]
[BHC2009]	(Brogan+Hunter+Cyganowski+, 2009)
Write:	<<[BHC2009] VLAN>>
N:	1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Use of archival VLA 7mm continuum data of NGC 6334 I(N).
Ref:	=2009ApJ...707....1B
by	BROGAN C.L. , HUNTER T.R., CYGANOWSKI C.J., INDEBETOUW R., BEUTHER H., MENTEN K.M., THORWIRTH S.
	Astrophys. J., 707, 1-23 (2009)
	Digging into NGC 6334 I(N): multiwavelength imaging of a massive protostellar cluster.
o	Calibrator J1720-355 is not in SIMBAD.
o	Table 1: <[BHC2009] VLAN> (No. VLA3), <[HBM2006b] I(N)-SMANa> (No. SMA1d) added.
=E=	Catalogue in electronic form as <J/ApJ/707/1/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHC2011]
[BHC2011]	(Brogan+Hunter+Cyganowski+, 2011)
Write:	<<[BHC2011] WW Core>> <<[BHC2011] NW CM2>> <<[BHC2011] Dark Core>>
N:	2+1+1
Object:	NH3 Core (SIMBAD class: denseCore = Dense Core)
Note:	Expanded VLA (EVLA) NH3 observations of the Extended Green Object EGO G035.03+0.35.
in source:	EGO G035.03+0.35
Ref:	=2011ApJ...739L..16B
by	BROGAN C.L. , HUNTER T.R., CYGANOWSKI C.J., FRIESEN R.K., CHANDLER C.J., INDEBETOUW R.
	Astrophys. J., 739L, 16 (2011)
	First results from a 1.3 cm expanded very large array survey of massive protostellar objects: G35.03+0.35.
o	Table 2: <[BHC2011] WW Core> (Nos NE, SW), <[BHC2011] Dark Core> N=1, <[BHC2011] NW CM2> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHC2016]
[BHC2016]	(Brogan+Hunter+Cyganowski+, 2016)
Write:	<<[BHC2016] MMN>> <<[BHC2016] MMNA>> <<[BHC2016] MM2A-core>> <<[BHC2016] MM2A-halo>> <<[BHC2016] CMN>>
N:	22
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 5cm, 1.5cm and 7mm and ALMA 3mm and 1.3mm continuum observations of N=22 radio sources in the field of the NGC 6334 I(N) protocluster. See also [HBM2006b]. In the format, CM stands for centimeter source.
in source:	NAME NGC 6334 I(N)
Ref:	=2016ApJ...832..187B
by	BROGAN C.L. , HUNTER T.R., CYGANOWSKI C.J., CHANDLER C.J., FRIESEN R., INDEBETOUW R.
	Astrophys. J., 832, 187-187 (2016)
	The massive protostellar cluster NGC 6334I at 220 au resolution: discovery of further multiplicity, diversity, and a hot multi-core.
o	Table 2, Fig. 1: <[BHC2016] MMN> (Nos 1-9), <[BHC2016] MM1A> N=9 among (Nos MM1A-MM1G, MM2B, MM4A), <[BHC2016] MM2A-core> N=1, <[BHC2016] MM2A-halo> N=1, <[BHC2016] CMN> (Nos CM1-CM2).
=E=	Catalogue in electronic form as <J/ApJ/832/187/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHD2006]
[BHD2006]	(Brunthaler+Henkel+De Blok+, 2006)
Write:	<<[BHD2006] NGC 6822 NN>>
N:	36
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	N=36 HII in NGC 6822 are studied.
in source:	NGC 6822
Ref:	=2006A&A...457..109B
by	BRUNTHALER A. , HENKEL C., DE BLOK W.J.G., REID M.J., GREENHILL L.J., FALCKE H.
	Astron. Astrophys., 457, 109-114 (2006)
	Water masers in the Local Group of galaxies.
o	Table A3: <[BHD2006] NGC 6822 NN> (Nos 1-36).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHD2015]
[BHD2015]	(Bahramian+Heinke+Degenaar+, 2015)
Write:	<<[BHD2015] CXNN>>
N:	4
Object:	Poss. LXMB (SIMBAD class: LowMassXBin_Candidate = Low Mass X-ray Binary Candidate)
Note:	Chandra ACIS-S observations of N=4 quiescent low-mass X-ray binaries (qLMXBs) in the globular cluster NGC 6266. See also CXOGlb.
in source:	NGC 6266
Ref:	=2015MNRAS.452.3475B
by	BAHRAMIAN A. , HEINKE C.O., DEGENAAR N., CHOMIUK L., WIJNANDS R., STRADER J., HO W.C.G., POOLEY D.
	Mon. Not. R. Astron. Soc., 452, 3475-3488 (2015)
	Limits on thermal variations in a dozen quiescent neutron stars over a decade.
o	p.3477: NGC 6397 U18 is a probablae misprint for U24 ([GHE2001b] U24 in Simbad, see associated references).
o	Table 2: <[BHD2015] CXNN> N=4 among (Nos CX4-CX16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHE2002]
[BHE2002]	(Billett+Hunter+Elmegreen, 2002)
Write:	<<[BHE2002] NGC NNNN NN>> <<[BHE2002] DDO NNN N>> <<[BHE2002] WLM N>> <<[BHE2002] Sex A N>>
N:	29+2+3+15+3+4+2+2
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST archives.
in source:	NGC 4214
in source:	NGC 2366
in source:	DDO 50 = Holmberg II
in source:	NGC 1705
in source:	DDO 168
in source:	DDO 165
in source:	DDO 221 = WLM Galaxy
in source:	NAME Sextans A
Ref:	=2002AJ....123.1454B
by	BILLETT O.H. , HUNTER D.A., ELMEGREEN B.G.
	Astron. J., 123, 1454-1475 (2002)
	Compact star clusters in nearby dwarf irregular galaxies.
o	Table 4: <[BHE2002] NGC 4214 NN> (Nos 1-29). Table 5: <[BHE2002] NGC 2366 N> (Nos 1-2). Table 6: <[BHE2002] DDO 50 N> (Nos 1-3). Table 7: <[BHE2002] NGC 1705 NN> (Nos 1-15). Table 8: <[BHE2002] DDO 168 N> (Nos 1-3). Table 9: <[BHE2002] DDO 165 N> (Nos 1-4). Table 10: <[BHE2002] WLM N> (Nos 1-2). Table 11: <[BHE2002] Sex A N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHE2009]
[BHE2009]	(Bianchi+Hutchings+Efremova+, 2009)
Write:	<<[BHE2009] GALEX JHHMMSS.ss+DDMMSS.s>>
N:	172
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	N=172 "FUV-NUV blue" QSOs, extracted from the GALEX MIS survey with complementary SDSS optical data.
Ref:	=2009AJ....137.3761B
by	BIANCHI L. , HUTCHINGS J.B., EFREMOVA B., HERALD J.E., BRESSAN A., MARTIN C.
	Astron. J., 137, 3761-3777 (2009)
	Ultraviolet quasi-stellar objects.
o	Tables 1-3: <[BHE2009] GALEX JHHMMSS.ss+DDMMSS.s> N=172+23+150.
=E=	Catalogue in electronic form as J/AJ/137/3761
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHF2006]
[BHF2006]	(Blakeslee+Holden+Franx+, 2006)
Write:	<<[BHF2006] RX J0152.7-1357 NNNNN>> <<[BHF2006] MS 1054-03 NNNN>>
N:	107+142
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	HST ACS observations of 2 clusters of galaxies.
in source:	RX J0152.7-1357 = ClG J0152-1357
in source:	ClG 1054-0321 = 1E 1054.4-0321
Ref:	=2006ApJ...644...30B
by	BLAKESLEE J.P. , HOLDEN B.P., FRANX M., ROSATI P., BOUWENS R.J., DEMARCO R., FORD H.C., HOMEIER N.L., ILLINGWORTH G.D., JEE M.J., MEI S., MENANTEAU F., MEURER G.R., POSTMAN M., TRAN K.-V.H.
	Astrophys. J., 644, 30-53 (2006)
	Clusters at half Hubble time: galaxy structure and colors in RX J0152.7-1357 and MS 1054-03.
o	Table 1: <[BHF2006] RX J0152.7-1357 NNNNN> N=107 among (Nos 543-57952). Table 2: <[BHF2006] MS 1054-03 NNNN> N=142 among (Nos 24-8456).
=E=	Catalogue in electronic form as J/ApJ/644/30
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHF2021]
[BHF2021]	(Barnes+Henshaw+Fontani+, 2021) (Not yet in Simbad)
Write:	<<[BHF2021] ANcNN>> <<[BHF2021] ANcN/N>> <<[BHF2021] ANcN/N/N>>
N:	82+12+2
Object:	Core (SIMBAD class: denseCore = Dense Core)
Note:	ALMA Band 3 (3mm) observations of N=96 cores in the infrared dark clouds [BT2009] A through J. See also [LTC2018].
Ref:	=2021MNRAS.503.4601B
by	BARNES A.T. , HENSHAW J.D., FONTANI F., PINEDA J.E., COSENTINO G., TAN J.C., CASELLI P., JIMENEZ-SERRA I., LAW C.Y., AVISON A., BIGIEL F., FENG S., KONG S., LONGMORE S.N., MOSER L., PARKER R.J., SANCHEZ-MONGE A., WANG K.
	Mon. Not. R. Astron. Soc., 503, 4601-4626 (2021)
	ALMA-IRDC: dense gas mass distribution from cloud to core scales.
o	Fig. 2, Tables A1-A2: <[BHF2021] ANcNN> N=82 among (Nos A1c3-A1c5 to J1c1-J1c3).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [BHF95]
[BHF95]	(Barth+Ho+Filippenko+, 1995)
Write:	<<[BHF95] NGC 1O97 NN>> <<[BHF95] NGC 6951 NN>>
N:	88+24
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST observations with WFPC2 and WFPC1. Table 1: format 'NGC 1097 NN', N=88 Table 2: format 'NGC 6951 NN', N=24
in source:	NGC 1097
in source:	NGC 6951
Ref:	=1995AJ....110.1009B
by	BARTH A.J. , HO L.C., FILIPPENKO A.V., SARGENT W.L.W.
	Astron. J., 110, 1009-1018 (1995)
	Hubble Space Telescope observations of circumnuclear star-forming rings in NGC 1097 and NGC 6951.
o	Table 1: <[BHF95] NGC 1097 NN> (Nos 1-88), Table 2: <[BHF95] NGC 6951 NN> (Nos 1-24)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHG2007]
[BHG2007]	(Brown+Haverkorn+Gaensler+, 2007)
Write:	<<[BHG2007] GLLL.ll+B.bb>>
N:	148
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Rotation measures of 148 extragalactic sources behind the SGP from the Southern Galactic Plane Survey (SGPS).
Ref:	=2007ApJ...663..258B
by	BROWN J.C. , HAVERKORN M., GAENSLER B.M., TAYLOR A.R., BIZUNOK N.S., McCLURE-GRIFFITHS N.M., DICKEY J.M., GREEN A.J.
	Astrophys. J., 663, 258-266 (2007)
	Rotation measures of extragalactic sources behind the southern Galactic plane: new insights into the large-scale magnetic field of the inner Milky Way.
o	Table 1: <[BHG2007] GLLL.ll+B.bb> N=148.
=E=	Catalogue in electronic form as J/ApJ/663/258
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHG2011]
[BHG2011]	(Bayliss+Hennawi+Gladders+, 2011)
Write:	<<[BHG2011] A1703 A>> <<[BHG2011] RXC J1327.0+0211 A>> <<[BHG2011] SDSS JHHMM+DDMM A>> <<[BHG2011] RCS2 JHHMM+DDMM A>> <<[BHG2011] GHO 132029+315500 A>> <<[BHG2011] A1703 AN>> <<[BHG2011] RXC J1327.0+0211 AN>> <<[BHG2011] SDSS JHHMM+DDMM AN>> <<[BHG2011] RCS2 JHHMM+DDMM AN>> <<[BHG2011] GHO 132029+315500 AN>> <<[BHG2011] JHHMMSS.sss+DDMMSS.sss>>
N:	26+69+13+1+149+256
Object:	Grav. lensed image of a G + Cluster of G + G
Note:	Gemini GMOS-North, NOT 2.5m telescope, WIYN 3.5m telescope and APO 3.5m telescope observations of strong-lensing cluster cores identified in the SDSS and RCS-2.
Ref:	=2011ApJS..193....8B
by	BAYLISS M.B. , HENNAWI J.F., GLADDERS M.D., KOESTER B.P., SHARON K., DAHLE H., OGURI M.
	Astrophys. J., Suppl. Ser., 193, 8 (2011)
	Gemini/GMOS spectroscopy of 26 strong-lensing-selected galaxy cluster cores.
o	Table 2: <[BHG2011] A1703 A>, <[BHG2011] RXC J1327.0+0211 A>, <[BHG2011] SDSS JHHMM+DDMM A>, <[BHG2011] RCS2 JHHMM+DDMM A>, <[BHG2011] GHO 132029+315500 A>, N=69. Table 3: <[BHG2011] SDSS JHHMM+DDMM> N=13, <[BHG2011] RCS2 JHHMM+DDMM> N=1. Table 4: <[BHG2011] A1703 AN>, <[BHG2011] RXC J1327.0+0211 AN>, <[BHG2011] SDSS JHHMM+DDMM AN>, <[BHG2011] RCS2 JHHMM+DDMM AN>, <[BHG2011] GHO 132029+315500 AN>, N=149. Table 4: <[BHG2011] JHHMMSS.sss+DDMMSS.sss> N=256.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHG83]
[BHG83]	(Beers+Huchra+Geller, 1983)
Write:	<<[BHG83] Clump A>> <<[BHG83] G NNN>>
N:	3+29
Object:	ClG + G (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	N=3 Clumps or sub-clusters in ACO 115. N=29 galaxies among about 270.
in source:	ACO 115
Ref:	=1983ApJ...264..356B
by	BEERS T.C. , HUCHRA J.P., GELLER M.J.
	Astrophys. J., 264, 356-363 (1983)
	Galaxy clusters with multiple components. II. Abell 115.
o	Table 1: <[BHG83] Clump A> (Nos A-C), <[BHG83] G NNN> N=29 among (Nos 1-212).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHG88]
[BHG88]	(Berkhuijsen+Humphreys+Ghigo+, 1988)
Write:	<<[BHG88] DD NNNN>>
N:	11438
Object:	* (SIMBAD class: Star)
Note:	Not all of the stars in the catalogue are necessarly members of M31 In field +39deg: N=1174, format '39 NNNN' In field +40deg: N=4962, format '40 NNNN' In field +41deg: N=5302, format '41 NNNN'
in source:	M 31 = NGC 224
Ref:	=1988A&AS...76...65B
by	BERKHUIJSEN E.M. , HUMPHREYS R.M., GHIGO F.D., ZUMACH W.
	Astron. Astrophys., Suppl. Ser., 76, 65-99 (1988)
	A catalogue of the brightest stars in the field of M 31.
o	Foreground stars not in SIMBAD
o	<[BHG88] DD NNNNN> N=11438
=E=	Catalogue in electronic form as II/144
=E=	Catalogue in electronic form as II/145
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHH2011]
[BHH2011]	(Basu-Zych+Hornschemeier+Hoversten+, 2011)
Write:	<<[BHH2011] AA>> <<[BHH2011] JHHMMSS.s+DDMMSS.s>>
N:	50+8
Object:	LBG + (UV) (SIMBAD class: UV = UV-emission Source)
Note:	Swift UVOT observations of the Chandra Deep Field South.
in source:	NAME CDFS
Ref:	=2011ApJ...739...98B
by	BASU-ZYCH A.R. , HORNSCHEMEIER A.E., HOVERSTEN E.A., LEHMER B., GRONWALL C.
	Astrophys. J., 739, 98 (2011)
	A search for Lyman break galaxies in the Chandra deep field south using Swift Ultraviolet/Optical telescope.
o	Tables 1-2: <[BHH2011] AA> (Nos A-Z, AA-XX), <[BHH2011] JHHMMSS.s+DDMMSS.s> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BHI
BHI	(Bootes void, HI)
Write:	<<BHI HHMM+DD>> <<BHI HHMM+DDMM>> <<BHI HHMMSS+DDMM>> <<BHI HHMMSS.s+DDMM>>
N:	19
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
in source:	NAME Bootes Void
Ref:	=1993AJ....105..464S
by	SZOMORU A. , VAN GORKOM J.H., GREGG M., DE JONG R.S.
	Astron. J., 105, 464-472 (1993)
	The first H I discovered galaxy in the Bootes void.
o	<BHI HHMM+DD> N=1, BHI 1517+39
Ref:	=1996AJ....111.2141S
by	SZOMORU A. , VAN GORKOM J.H., GREGG M.D.
	Astron. J., 111, 2141-2149 (1996)
	An H I survey of the Bootes void. I. The data.
o	Plates 79-120: <BHI HHMM+DDMM>, <BHI HHMMSS+DDMM>, <BHI HHMMSS.s+DDMM> N=17
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BHI96]
[BHI96]	(Brandt+Halpern+Iwasawa, 1996)
Write:	<<[BHI96] JHHMMSS.s+DDMMSS.s>> <<[BHI96] X-N>>
N:	13
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT PSPC and HRI observations
in source:	NGC 1672
Ref:	=1996MNRAS.281..687B
by	BRANDT W.N. , HALPERN J.P., IWASAWA K.
	Mon. Not. R. Astron. Soc., 281, 687-695 (1996)
	ROSAT PSPC and HRI observations of the composite starburst/Seyfert 2 galaxy NGC 1672.
o	Table 1: <[BHI96] JHHMMSS.s-DDMMSS.s> N=10 among which 6 are also: <[BHI96] X-N> (Nos X-1 to X-6)
Ref:	=2000AJ....119..612D
by	DE NARAY P.J. , BRANDT W.N., HALPERN J.P., IWASAWA K.
	Astron. J., 119, 612-619 (2000)
	New X-ray constraints on starburst and Seyfert activity in the barred spiral galaxy NGC 1672.
o	Table 1: <[BHI96] X-N> (Nos X-7 to X-9) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BHJ
BHJ	(Blaauw+Hiltner+Johnson)
Write:	<<BHJ NNaa>>
N:	91
Object:	* in Assoc. (SIMBAD class: Star)
Note:	Stars in the Cep OB 3- association. (Nos 1-83), No.8 have two components, the brightest component 'NNbr' and the faintest 'NNft'.
in source:	NAME ASS CEP OB 3-
Ref:	=1959ApJ...130...69B
by	BLAAUW A. , HILTNER W.A., JOHNSON H.L.
	Astrophys. J., 130, 69-79 (1959)
	Photoelectric photometry of the association III Cephei.
o	(Erratum) 1960 ApJ 131, P. 327
o	T.1: cross-id. Munch not in Simbad
o	Table 1: <BHJ NNaa> (Nos 1-83) among which 8 have two components 'NNbr' and 'NNft'
Origin	of the Acronym: L = Found in the literature
History	of this Acronym: replaces ASS Cep OB 3 (oct. 1996)
Details on Acronym: BHJ
BHJ	(Blaauw+Hiltner+Johnson)
Write:	<<BHJ NN-NNN>>
N:	1056
Object:	* (SIMBAD class: Star)
Note:	Stars in a field containing at least one star 'BHJ NN', NN 1st part of the format) total number of * in the work = 1056 in 18 selected fields
Ref:	=1995A&AS..114..489J
by	JORDI C. , GALADI-ENRIQUEZ D., TRULLOLS E., LAHULLA F.
	Astron. Astrophys., Suppl. Ser., 114, 489-497 (1995)
	UBVRI-CCD photometry of Cepheus OB3 association.
o	<BHJ NN-NNN> N=1056
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BHJ2002]
[BHJ2002]	(Benedict+Howell+Jorgensen+, 2002)= (NRC)
Write:	<<[BHJ2002] NRC NN>>
N:	76
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 images of NGC 4314.
in source:	NGC 4314
Ref:	=2002AJ....123.1411B
by	BENEDICT G.F. , HOWELL D.A., JORGENSEN I., KENNEY J.D.P., SMITH B.J.
	Astron. J., 123, 1411-1432 (2002)
	NGC 4314. IV. Photometry of star clusters with the Hubble space telescope: history of star formation in the vicinity of a nuclear ring.
o	Table 2: <[BHJ2002] NRC NN> (Nos 1-76).
=E=	Catalogue in electronic form as J/AJ/123/1411
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHJ77]
[BHJ77]	(Baker+Haslam+Jones+, 1977)= BHJW
Write:	<<[BHJ77] I-NN>> <<[BHJ77] II-N>>
N:	14+5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 4, I: N=14 sources from Harten (reference not published). Table 4, II: N=5 further discrete sources from the authors. See also [HG90b].
in source:	IC 342
Ref:	=1977A&A....59..261B
by	BAKER J.R. , HASLAM C.G.T., JONES B.B., WIELEBINSKI R.
	Astron. Astrophys., 59, 261-266 (1977)
	Radio continuum observations of the spiral galaxy IC 342.
o	Table 4: <[BHJ77] I-NN> (Nos I-1 to I-14), <[BHJ77] II-N> (Nos II-1 to II-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHJ93]
[BHJ93]	(Benedict+Higdon+Jefferys+, 1993)= ([HJD93])
Write:	<<[BHJ93] NN>>
N:	14
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
in source:	NGC 4314
Ref:	=1993AJ....105.1369B
by	BENEDICT G.F. , HIGDON J.L., JEFFERYS W.H., DUNCOMBE R., HEMENWAY P.D., SHELUS P.J., WHIPPLE A.L., NELAN E., STORY D., McARTHUR B., McCARTNEY J., FRANZ O.G., FREDRICK L.W., VAN ALTENA W.F.
	Astron. J., 105, 1369-1377 (1993)
	NGC 4314. II. Hubble Space Telescope I-band surface photometry of the nuclear region.
o	Table 1: <[BHJ93] NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BHJW
BHJW	(Baker+Haslam+Jones+Wielebinski)
*****	Avoid the usage of BHJW, prefer [BHJ77]
Origin	of the Acronym: L (1980A&A....90..246I)
Details on Acronym: [BHK2005]
[BHK2005]	(Bastian+Hempel+Kissler-Patig+, 2005)
Write:	<<[BHK2005] NNN>>
N:	118
Object:	Poss. GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	VLT-FORSI images (original observations and archival material) of NGC 6872, to study the star cluster population. Additional Halpha Fabry-Perot observations from C.J. Mihos (see 1993ApJ...418...82M).
Ref:	=2005A&A...435...65B
by	BASTIAN N. , HEMPEL M., KISSLER-PATIG M., HOMEIER N.L., TRANCHO G.
	Astron. Astrophys., 435, 65-75 (2005)
	The star cluster population in the tidal tails of NGC 6872.
o	Table 2: <[BHK2005] NNN> N=118 among (Nos 2-456).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHK2021]
[BHK2021]	(Bahramian+Heinke+Kennea+, 2021) (Not yet in Simbad)
Write:	<<[BHK2021] SBS XNNN>>
N:	104
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Swift XRT observations of N=104 X-ray sources, as part of the Swft Galactic Bulge survey.
in source:	NAME Galactic Bulge
Ref:	=2021MNRAS.501.2790B
by	BAHRAMIAN A. , HEINKE C.O., KENNEA J.A., MACCARONE T.J., EVANS P.A., WIJNANDS R., DEGENAAR N., IN'T ZAND J.J.M., SHAW A.W., RIVERA SANDOVAL L.E., McCLURE S., TETARENKO A.J., STRADER J., KUULKERS E., SIVAKOFF G.R.
	Mon. Not. R. Astron. Soc., 501, 2790-2809 (2021)
	The Swift bulge survey: motivation, strategy, and first X-ray results.
o	Catalog, col(1): <[BHK2021] SBS XNNN> N=104 among (Nos X1-X807) = Catalog, col(2): <SWIFT JHHMMSS.s+DDMMSS> N=104.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHK94]
[BHK94]	(Bershady+Hereld+Kron+, 1994)
*****	Avoid the usage of [BHK94], prefer [K80]
Origin	of the Acronym: L (NED)
Details on Acronym: [BHL94]
[BHL94]	(Bridle+Hough+Lonsdale+, 1994)
Write:	<<[BHL94] 3C NNN.N A>> <<[BHL94] 3C NNN.N AN>>
N:	152
Object:	Knot (SIMBAD class: Radio = Radio Source)
Note:	Figs 1 to 36: Maps of knots in 13 QSO from the 3CR catalogue.
in source:	3C 9
in source:	3C 68.1
in source:	3C 175
in source:	3C 204
in source:	3C 208
in source:	3C 215
in source:	3C 249.1
in source:	3C 263
in source:	3C 334
in source:	3C 336
in source:	3C 351
in source:	3C 432
in source:	3C 47
Ref:	=1994AJ....108..766B
by	BRIDLE A.H. , HOUGH D.H., LONSDALE C.J., BURNS J.O., LAING R.A.
	Astron. J., 108, 766-820 (1994)
	Deep VLA imaging of twelve extended 3CR quasars.
o	Figs 1 to 36: <[BHL94] 3C NNN A>, <[BHL94] 3C NNN AN>, <[BHL94] 3C NNN.N A>, <[BHL94] 3C NNN.N AN>, N=152
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHM2000]
[BHM2000]	(Bonifacio+Hill+Molaro+, 2000)= (Sgr)
Write:	<<[BHM2000] NNN>>
N:	2
Object:	Giant * (SIMBAD class: Star)
Note:	N=2 giant stars in Sgr dwarf galaxy, from a unpublished list of Bonifacio. See also [SL95] and [MBC98].
in source:	NAME SDG = NAME Sgr Dwarf Galaxy
Ref:	=2000A&A...359..663B
by	BONIFACIO P. , HILL V., MOLARO P., PASQUINI L., DI MARCANTONIO P., SANTIN P.
	Astron. Astrophys., 359, 663-668 (2000)
	First results of UVES at VLT: abundances in the Sgr dSph.
o	Bonifacio writes: objects in Table 1 are neither [SL95] nor [MBC98] objects.
o	Table 1: <[BHM2000] NNN> (Nos 139, 143).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHM2006]
[BHM2006]	(Bowen+Hennawi+Menard+, 2006)
Write:	<<[BHM2006] QSO JHHMM+DDMMA abs N.NNNN>>
N:	4
Object:	Absorber
Note:	Search for ALS in SDSS spectra of background QSO in QSO pair.
Ref:	=2006ApJ...645L.105B
by	BOWEN D.V. , HENNAWI J.F., MENARD B., CHELOUCHE D., INADA N., OGURI M., RICHARDS G.T., STRAUSS M.A., VANDEN BERK D.E., YORK D.G.
	Astrophys. J., 645, 105-108 (2006)
	QSO absorption lines from QSOS.
o	Table 1: <[BHM2006] QSO JHHMM+DDMMA abs N.NNNN> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHM2009]
[BHM2009]	(Bouy+Huelamo+Martin+, 2009)= (SigOri-MAD) = (SigOri-SofI)
Write:	<<[BHM2009] SigOri-MAD-NN>> <<[BHM2009] SigOri-SofI-NNN>>
N:	36+398
Object:	(NIR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	VLT Multi-Conjugate Adaptive Optics Demonstrator (MAD) images of the core of sigma-Orionis cluster, complemented by archival NTT/SofI Ks-band images and Spitzer IRAC and MIPS mid-infrared images.
in source:	NAME sig Ori Cluster
Ref:	=2009A&A...493..931B
by	BOUY H. , HUELAMO N., MARTIN E.L., MARCHIS F., BARRADO Y NAVASCUES D., KOLB J., MARCHETTI E., PETR-GOTZENS M.G., STERZIK M., IVANOV V.D., KOEHLER R., NUERNBERGER D.
	Astron. Astrophys., 493, 931-946 (2009)
	A deep look into the cores of young clusters. I. σ-Orionis.
o	Fig. 2, Table 3: <[BHM2009] SigOri-MAD-NN> (Nos 1-36). Table 8: <[BHM2009] SigOri-SofI-NNN> (Nos 1-398).
=E=	Catalogue in electronic form as J/A+A/493/931
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHM2011]
[BHM2011]	(Burgarella+Heinis+Magdis+, 2011)
Write:	<<[BHM2011] JHHMMSS.s+DDMMSS.s>>
N:	13
Object:	LBG (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Herschel, Spitzer, and GALEX observations of the GOODS-North field.
in source:	NAME GOODS North Field
Ref:	=2011ApJ...734L..12B
by	BURGARELLA D. , HEINIS S., MAGDIS G., AULD R., BLAIN A., BOCK J., BRISBIN D., BUAT V., CHANIAL P., CLEMENTS D.L., COORAY A., EALES S., FRANCESCHINI A., GIOVANNOLI E., GLENN J., GONZALEZ SOLARES E.A., GRIFFIN M., HWANG H.S., ILBERT O., MARCHETTI L., MORTIER A.M.J., OLIVER S.J., PAGE M.J., PAPAGEORGIOU A., PEARSON C.P., PEREZ-FOURNON I., POHLEN M., RAWLINGS J.I., RAYMOND G., RIGOPOULOU D., RODIGHIERO G., ROSEBOOM I.G., ROWAN-ROBINSON M., SCOTT D., SEYMOUR N., SMITH A.J., SYMEONIDIS M., TUGWELL K.E., VACCARI M., VIEIRA J.D., VIERO M., VIGROUX L., WANG L., WRIGHT G.
	Astrophys. J., 734L, 12 (2011)
	HerMES: Lyman break galaxies individually detected at 0.7 ≤ z ≤ 2.0 in GOODS-N with Herschel/SPIRE.
o	Table 1: <[BHM2011] JHHMMSS.s+DDMMSS.s> N=13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHM2012]
[BHM2012]	(Bielby+Hill+Metcalfe+, 2012)= ([BHM2012a])
Write:	<<[BHM2012] WHDF-LAB-NN>> <<[BHM2012] WHDFCH-NNN>>
N:	11+15
Object:	(submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	APEX LABOCA 870µm observations of N=11 submillimeter sources in the William Herschel Deep Field (WHDF). Magellan-1 6.5m telescope LDSS2 spectroscopy of N=15 quasars in the WHDF. Format WHDFCH-NNN refers to the sources listed in Table 2 of 2012MNRAS.419.1315B and the nomenclature originates from Vallbe-Mumbru (2004, PhD thesis, Durham Univ.).
in source:	NAME Herschel Deep Field
Ref:	=2012MNRAS.419.1315B
by	BIELBY R.M. , HILL M.D., METCALFE N., SHANKS T.
	Mon. Not. R. Astron. Soc., 419, 1315-1323 (2012)
	Submillimetre observations of X-ray active galactic nuclei in the william Herschel deep field.
o	Table 1: <[BHM2012] WHDF-LAB-NN> (Nos 01-11). Table 2: <[BHM2012] WHDFCH-NNN> N=15 among (Nos 005-113).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHM2012a]
[BHM2012a]	(Bielby+Hill+Metcalfe+, 2012)
*****	Avoid the usage of [BHM2012a], prefer [BHM2012]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHM2012b]
[BHM2012b]	(Barsony+Haisch+Marsh+, 2012)
Write:	<<[BHM2012b] NNN>>
N:	948
Object:	Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Stat:	is completely incorporated in Simbad
Note:	AAT IRIS2 observations of N=948 candidate YSOs in the ρ Oph cluster.
in source:	NAME rho Oph Cloud
Ref:	=2012ApJ...751...22B
by	BARSONY M. , HAISCH K.E., MARSH K.A., McCARTHY C.
	Astrophys. J., 751, 22 (2012)
	A significant population of candidate new members of the ρ Ophiuchi cluster.
o	Table 3: <[BHM2012b] NNN> (Nos 1-948).
=E=	Catalogue in electronic form as J/ApJ/751/22
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BHR
BHR	(Bourke+Hyland+Robinson)
Write:	<<BHR NNN>>
N:	169
Object:	Dark Cloud (SIMBAD class: Globule = Globule (low-mass dark cloud))
Stat:	is completely incorporated in Simbad
Ref:	=1995MNRAS.276.1052B
by	BOURKE T.L. , HYLAND A.R., ROBINSON G.
	Mon. Not. R. Astron. Soc., 276, 1052-1066 (1995)
	Studies of star formation in isolated small dark clouds - I. A catalogue of southern Bok globules : optical and IRAS properties.
o	<BHR NNN> (Nos 1-169)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BHR2005]
[BHR2005]	(Bochanski+Hawley+Reid+, 2005)
Write:	<<[BHR2005] NNN>> <<[BHR2005] FFF-NNN>>
N:	574+31
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	2.5m DuPont telescope at Las Campanas. Use of 2MASS and USNO-B archival data. Spectroscopic observations of 574 M dwarfs and 31 K dwarfs.
Ref:	=2005AJ....130.1871B
by	BOCHANSKI J.J. , HAWLEY S.L., REID I.N., COVEY K.R., WEST A.A., TINNEY C.G., GIZIS J.E.
	Astron. J., 130, 1871-1879 (2005)
	Spectroscopic survey of M dwarfs within 100 parsecs of the Sun.
o	(Erratum) erratum vol. 131, p.3136 (2006)
o	Table 1: <[BHR2005] NNN> (Nos 1-574) = <[BHR2005] FFF-NNN> N=574. Table 3: <[BHR2005] FFF-NNN> N=31.
=E=	Catalogue in electronic form as J/AJ/130/1871
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHR99]
[BHR99]	(Beuermann+Hessman+Reinsch+, 1999)
Write:	<<[BHR99] A>>
N:	5
Object:	* + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	FORS1 VLT observations. Fig.3: Objects in the field of GRB 990510. (Nos A-D) are stars, (Nos A-C) identical to [CLG99] A to C. (No. E) is a possible galaxy. See also [CLG99] and [PU99].
Ref:	=1999A&A...352L..26B
by	BEUERMANN K. , HESSMAN F.V., REINSCH K., NICKLAS H., VREESWIJK P.M., GALAMA T.J., ROL E., VAN PARADIJS J., KOUVELIOTOU C., FRONTERA F., MASETTI N., PALAZZI E., PIAN E.
	Astron. Astrophys., 352, 26-30 (1999)
	VLT observations of GRB 990510 and its environment.
o	Table 1: Star 3 = [PU99] Star 3.
o	Fig.3, Table 1: <[BHR99] A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHS2000]
[BHS2000]	(Brandt+Hornschemeier+Schneider+, 2000)
Write:	<<[BHS2000] N>> <<[BHS2000] AG N>> <<[BHS2000] IN>> <<[BHS2000] JHHMMSS.s+DDMMSS.s>>
N:	9+1+1+1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of N=9 sources in the field of the ClG CRSS J0030.5+2618, (Nos 1-9). N=2 other sources are found: 'AG 1' found on ASCA Grade filtering, 'I3' found on ACIS CCD I3. The authors also detect a sources at 00 30 57.8 +26 17 44.3 (2000) lying at about 19" from the edge of S3. Finding charts figs 1, 2.
Ref:	=2000AJ....119.2349B
by	BRANDT W.N. , HORNSCHEMEIER A.E., SCHNEIDER D.P., GARMIRE G.P., CHARTAS G., HILL G.J., MacQUEEN P.J., TOWNSLEY L.K., BURROWS D.N., KOCH T.S., NOUSEK J.A., RAMSEY L.W.
	Astron. J., 119, 2349-2359 (2000)
	Observations of faint, hard-band X-ray sources in the field of CRSS J0030.5+2618 with the Chandra X-ray observatory and the Hobby-Eberly telescope.
o	Table 1: <[BHS2000] N> (Nos 1-9), <[BHS2000] AG 1> N=1, <[BHS2000] I 3> N=1. P.2350, note: <[BHS2000] JHHMMSS.s+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHS71]
[BHS71]	(Berkhuijsen+Haslam+Salter, 1971)= (Loop)
Write:	<<[BHS71] Loop R>>
N:	6
Object:	Poss. Gal. SNR (SIMBAD class: SNRemnant_Candidate = SuperNova Remnant Candidate)
Stat:	is completely incorporated in Simbad
Note:	Loop V was first found in ref. 1973Ap&SS..20..111E but the nomenclature in this ref. is somewhat confusing.
Ref:	=1971A&A....14..252B
by	BERKHUIJSEN E.M. , HASLAM C.G.T., SALTER C.J.
	Astron. Astrophys., 14, 252-262 (1971)
	Are the galactic loops supernova remnants ?
o	<[BHS71] Loop R> (Nos I-IV)
Ref:	=1976ApJ...208..718N
by	NARANAN S. , SHULMAN S., FRIEDMAN H., FRITZ G.
	Astrophys. J., 208, 718-726 (1976)
	Soft X-ray emission in Eridanus: an old supernova remnant ?
o	<[BHS71] Loop R> (No. V) added
Ref:	=2007MNRAS.376..634B
by	BORKA V.
	Mon. Not. R. Astron. Soc., 376, 634-644 (2007)
	Spectral indices of Galactic radio loops between 1420, 820 and 408 MHz.
o	Table 1: <[BHS71] Loop R> (No. VI) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHS95]
[BHS95]	(Beauchamp+Hardy+Suntzeff+, 1995)
Write:	<<[BHS95] C2 NNN>> <<[BHS95] C4 NNNN>>
N:	9+39
Object:	* in Cl* (SIMBAD class: Star)
Note:	Table 5: format 'C2 NNN', N=9 * in Cluster 2 among (Nos 4-823) Table 6: format 'C4 NNNN', N=39 * in Cluster 4 among (Nos 177-5029)
in source:	NAME Fornax 2
in source:	NAME Fornax 4
Ref:	=1995AJ....109.1628B
by	BEAUCHAMP D. , HARDY E., SUNTZEFF N.B., ZINN R.
	Astron. J., 109, 1628-1644 (1995)
	Color-magnitude diagrams for clusters 2 and 4, and the field in the Fornax dwarf spheroidal galaxy.
o	C2 = NAME FORNAX 2, C4 = NAME FORNAX 4
o	Table 5: <[BHS95] C2 NNN> N=9 among (Nos 4-823), Table 6: <[BHS95] C4 NNNN> N=39 among (Nos 177-5029)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHS98]
[BHS98]	(Briceno+Hartmann+Stauffer, 1998)= (MHO)
Write:	<<[BHS98] MHO NN>>
N:	12
Object:	T Tau * (SIMBAD class: TTauri* = T Tauri Star)
Stat:	is completely incorporated in Simbad
Note:	In the format, 'MHO' stands for Mount Hopkins Observatory.
in source:	NAME Taurus Cloud
Ref:	=1998AJ....115.2074B
by	BRICENO C. , HARTMANN L., STAUFFER J., MARTIN E.
	Astron. J., 115, 2074-2091 (1998)
	A search for very low mass pre-main-sequence stars in Taurus.
o	Group in Taurus = [GHK93] Group I, II, IV, VI.
o	Table 4: <[BHS98] MHO NN> (Nos 1-12)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHT2019]
[BHT2019]	(Brogan+Hunter+Towner+, 2019)
Write:	<<[BHT2019] G358.93-00.03 MMN>>
N:	8
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	SMA and ALMA band 5, 6, 7 observations of N=8 (sub)millimeter continuum sources in the field of the star-forming region GAL 358.93-00.03.
in source:	GAL 358.93-00.03
Ref:	=2019ApJ...881L..39B
by	BROGAN C.L. , HUNTER T.R., TOWNER A.P.M., McGUIRE B.A., MacLEOD G.C., GURWELL M.A., CYGANOWSKI C.J., BRAND J., BURNS R.A., CARATTI O GARATTI A., CHEN X., CHIBUEZE J.O., HIRANO N., HIROTA T., KIM K.-T., KRAMER B.H., LINZ H., MENTEN K.M., REMIJAN A., SANNA A., SOBOLEV A.M., SRIDHARAN T.K., STECKLUM B., SUGIYAMA K., SURCIS G., VAN DER WALT J., VOLVACH A.E., VOLVACH L.N.
	Astrophys. J., 881L, 39-39 (2019)
	Sub-arcsecond (sub)millimeter imaging of the massive protocluster G358.93-0.03: discovery of 14 new methanol maser lines associated with a hot core.
o	Fig. 1, Table 2: <[BHT2019] G358.93-00.03 MMN> (Nos MM1-MM8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHT89]
[BHT89]	(Burns+Hayward+Thronson+, 1989) (Not yet in Simbad)
Write:	<<[BHT89] Loop A>>
N:	2
Object:	Em. Loop (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=2 loops of emission in the H image of AFGL 2591.
in source:	RAFGL 2591
Ref:	=1989AJ.....98..659B
by	BURNS M.S. , HAYWARD T.L., THRONSON H.A.Jr, JOHNSON P.E.
	Astron. J., 98, 659-664 (1989)
	Imaging polarimetry of AFGL 2591 and its associated reflection nebula.
o	Fig.4: <[BHT89] Loop A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHW2010]
[BHW2010]	(Becker+Helfand+White+, 2010)
Write:	<<[BHW2010] GLL.llll+B.llll>>
N:	39
Object:	Variable Radio Source (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA observations in the Galactic Plane.
Ref:	=2010AJ....140..157B
by	BECKER R.H. , HELFAND D.J., WHITE R.L., PROCTOR D.D.
	Astron. J., 140, 157-166 (2010)
	Variable radio sources in the galactic plane.
o	Table 2: <[BHW2010] GLL.llll+B.llll> N=39.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHW2021]
[BHW2021]	(Becker+Hurley-Walker+Weinberger+, 2021)
Write:	<<[BHW2021] NN>>
N:	11
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	N=11 X-ray sources in the field of SNR G249.5+24.5. Use of the first eROSITA all-sky survey eRASS1 and of archival ROSAT all-sky survey (RASS).
Ref:	=2021A&A...648A..30B
by	BECKER W. , HURLEY-WALKER N., WEINBERGER C., NICASTRO L., MAYER M.G.F., MERLONI A., SANDERS J.
	Astron. Astrophys., 648A, 30-30 (2021)
	Hoinga: a supernova remnant discovered in the SRG/eROSITA All-Sky Survey eRASS1.
o	Table 1: <[BHW2021] NN> (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BHW93]
[BHW93]	(Becker+Henkel+Wilson+, 1993)
Write:	<<[BHW93] HHMMSS.s+DDMMSS>>
N:	2
Object:	H2O Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	Effelsberg 100m telescope observations of IC 10 to search for H2O masers.
in source:	IC 10
Ref:	=1993A&A...268..483B
by	BECKER R. , HENKEL C., WILSON T.L., WOUTERLOOT J.G.A.
	Astron. Astrophys., 268, 483-490 (1993)
	H2O masers in nearby irregular galaxies.
o	Paragr. 3: <[BHW93] HHMMSS.s+DDMMSS> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Bi
Bi	(Bidelman) (Not yet in Simbad)
*****	Avoid the usage of Bi, prefer [B54]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BI
BI	(Brunet+Imbert+)= (Bru)
Write:	<<BI NNN>>
N:	272
Object:	O-B2 * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Finding charts.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1975A&AS...21..109B
by	BRUNET J.P. , IMBERT M., MARTIN N., MIANES P., PREVOT L., REBEIROT E., ROUSSEAU J.
	Astron. Astrophys., Suppl. Ser., 21, 109-136 (1975)
	Recherches dans le Grand Nuage de Magellan. I. Un catalogue de 272 etoiles O-B2 nouvelles.
o	Catalogue: <BI NNN> (Nos 1-272)
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [BI2006]
[BI2006]	(Biggs+Ivison, 2006)
Write:	<<[BI2006] JHHMMSS.sss+DDMMSS.ss>>
N:	506+537+200
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Deep VLA 1.4GHz observations of 3 fields.
in source:	NAME Lockman Hole
in source:	NAME HDFN
in source:	ELAIS N2
Ref:	=2006MNRAS.371..963B
by	BIGGS A.D. , IVISON R.J.
	Mon. Not. R. Astron. Soc., 371, 963-971 (2006)
	A catalogue of µJy radio sources in northern legacy fields.
o	Table 2: <[BI2006] JHHMMSS.sss+DDMMSS.ss> N=506+537+200.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BI2008]
[BI2008]	(Biggs+Ivison, 2008)
Write:	<<[BI2008] SMGNN>> <<[BI2008] CNN>>
N:	12+21
Object:	(smm) + (Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	MERLIN and VLA 1.4GHz observations of the Lockman Hole to search for SubMillimeter Galaxies. N=12 SMG are found. Control sample of N=21 radio sources.
in source:	NAME Lockman Hole
Ref:	=2008MNRAS.385..893B
by	BIGGS A.D. , IVISON R.J.
	Mon. Not. R. Astron. Soc., 385, 893-904 (2008)
	High-resolution radio observations of submillimetre galaxies.
o	Figs 1, 2, Table 1: <[BI2008] SMGNN> (Nos SMG01 to SMG12). Figs 1, 3, Table 2: <[BI2008] CNN> (Nos C01-C21).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BIB2006]
[BIB2006]	(Bouwens+Illingworth+Blakeslee+, 2006)
Write:	<<[BIB2006] JHHMMSS.ss+DDMMSS.s>> <<[BIB2006] HDFN-MSSssMMSSs>> <<[BIB2006] CDFS-MSSssMMSSs>> <<[BIB2006] UDF-SSssMSSs>> <<[BIB2006] HUDF-SSssMSSs>> <<[BIB2006] HUDFP1-MSSssMMSSs>> <<[BIB2006] HUDFP2-MSSssMMSSs>>
N:	581
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Search for i-dropouts in deep, wide-area HST ACS fields.
in source:	NAME HDFN
in source:	NAME HUDF
in source:	NAME CDFS
Ref:	=2006ApJ...653...53B
by	BOUWENS R.J. , ILLINGWORTH G.D., BLAKESLEE J.P., FRANX M.
	Astrophys. J., 653, 53-85 (2006)
	Galaxies at z ~ 6: the UV luminosity function and luminosity density from 506 HUDF, HUDF parallel ACS field, and GOODS i-dropouts.
o	Table 2: <[BIB2006] JHHMMSS.ss+DDMMSS.s> N=43. Table 6: <[BIB2006] HDFN-MSSssMMSSs> N=9+151, <[BIB2006] CDFS-MSSssMMSSs> N=10+181, <[BIB2006] UDF-SSssMSSs> N=1. Table 4: <[BIB2006] HUDF-SSssMSSs> N=128. Table 5: <[BIB2006] HUDFP1-MSSssMMSSs> N=54, <[BIB2006] HUDFP2-MSSssMMSSs> N=14.
=E=	Catalogue in electronic form as J/ApJ/653/53
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BIC
BIC	(Benaglia+Ishwara-Chandra) (Not yet in Simbad)
Write:	<<BIC 325-NNNN>> <<BIC 610-NNNN>>
N:	1048+2796
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	GMRT 325 and 610 MHz observations of N=1048+2796 radio sources respectively, in the center of the Cygnus rift.
in source:	NAME Cyg Rift
Ref:	=2020A&A...642A.136B
by	BENAGLIA P. , ISHWARA-CHANDRA C.H., INTEMA H., COLAZO M.E., GAIKWAD M.
	Astron. Astrophys., 642A, 136-136 (2020)
	Cygnus survey with the Giant Metrewave Radio Telescope at 325 and 610 MHz: the catalog.
o	Table 3: <BIC 325-NNNN> (Nos 0001-1048). Table 4: <BIC 610-NNNN> (Nos 0001-2796).
=E=	Catalogue in electronic form as <J/A+A/642/A136/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Bica
Bica	(Bica+)
Write:	<<Cl Bica N>>
Object:	Poss. Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	See also [BBD2003].
in source:	Ass Cyg OB 2 = NAME VI CYG
Ref:	=2003A&A...405..991B
by	BICA E. , BONATTO C., DUTRA C.M.
	Astron. Astrophys., 405, 991-998 (2003)
	Does Cyg OB2 harbour any open cluster?
o	Do 44 = Cl Dolidze 44.
o	<[BBD2003] Object N> (Nos 1-3).
Origin	of the Acronym: L (2006A&A...446..949D)
Details on Acronym: [BIF2008]
[BIF2008]	(Bouwens+Illingworth+Franx+, 2008)= (CDFS) = (HDFN) = (NICPAR1) = (NICPAR2) = (UDF)
Write:	<<[BIF2008] HDFN-MMSS-MMSS>> <<[BIF2008] NICPARN-MMSS-MMSS>> <<[BIF2008] CDFS-MMSS-MMSS>> <<[BIF2008] UDF-MMSS-MMSS>>
N:	5
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST NICMOS, VLT ISAAC, and Subaru MIRCS observations of the HUDF and GOODS fields. N=9 z-dropout candidate galaxies. See also [BTI2004] and [BIT2005].
Ref:	=2008ApJ...686..230B
by	BOUWENS R.J. , ILLINGWORTH G.D., FRANX M., FORD H.
	Astrophys. J., 686, 230-250 (2008)
	z ~ 7-10 galaxies in the HUDF and GOODS fields: UV luminosity functions.
o	Table 2: Objects UDF-NNN-NNNN are [BTI2004] UDF-NNN-NNNN in SIMBAD.
o	Table 2: <[BIF2008] HDFN-MMSS-MMSS>, <[BIF2008] NICPAR2-MMSS-MMSS>, <[BIF2008] NICPAR1-MMSS-MMSS>, <[BIF2008] CDFS-MMSS-MMSS>, <[BIF2008] UDF-MMSS-MMSS>, N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BIG
BIG	(Byurakan, IR Galaxy)
Write:	<<BIG NNNa>>
N:	?
Object:	G (SIMBAD class: Galaxy)
Note:	FBS IRAS galaxies. Stars and galaxies are simultaneously included in the four first refs, and a general numbering was made. See [M97c], BIS. 2000Ap.....43..309M: "179 IR sources were identified with extragalactic objects in the first refs, the numbering continues from the number 180. The galaxies published earlier will be designated BIG 1 to 179 in the order of publication".
Ref:	=1997Ap.....40....1M
by	MICKAELIAN A.M.
	Astrophysics, 40, 1-9 (1997)
	Optical identification of 100 IRAS point sources at high galactic latitude.
o	Galaxies 'BIG NN' and stars 'BIS NN' are not numbered here, they are respectively the galaxies and the stars included in [M97c] NNN objects.
o	Table 1: <[M97c] NNN> (Nos 1-100). Table 1: <BIG NN> N=? Table 1: <BIS NN> (Nos 1-61)?
Ref:	=1997Ap.....40..379M
by	MICKAELIAN A.M. , GIGOYAN K.S., RUSSEIL D.
	Astrophysics, 40, 379-389 (1997)
	Optical identification of IRAS point sources on the basis of low-dispersion FBS spectra. II.
o	Galaxies 'BIG NN' are not numbered here, they are added to the galaxies in the first '[M97c]' reference: 1997Ap.....40....1M.
o	Table 1: <[M97c] NNNa> (Nos 101-158) N=68. Table 1: <BIG NNN> N=?
Ref:	=1998Ap.....41..161M
by	MICKAELIAN A.M. , GIGOYAN K.S.
	Astrophysics, 41, 161-169 (1998)
	Optical identification of IRAS point sources on the basis of low-dispersion FBS spectra. III.
o	Galaxies 'BIG NNN' are not numbered here, they are added to the galaxies in the first '[M97c]' references.
o	Table 1: <[M97c] NNNa> (Nos 159-206) N=62. Table 1: <BIG NNN> N=?
Ref:	=1998Ap.....41..232M
by	MICKAELIAN A.M. , GIGOYAN K.S.
	Astrophysics, 41, 232-238 (1998)
	Optical identification of IRAS point sources on the basis of low-dispersion FBS spectra. IV.
o	Galaxies 'BIG NNN' are not numbered here, they are added to the galaxies in the first '[M97c]' references.
o	Table 1: <[M97c] NNNa> (Nos 207-240) N=51. Table 1: <BIG NNN> N=?
Ref:	=2000Ap.....43..309M
by	MICKAELIAN A.M.
	Astrophysics, 43, 309-321 (2000)
	Optical identification of IRAS point sources. Galaxies. V.
o	BIG numbering (Nos 1-179) are the galaxies in 1997Ap.....40....1M, 1997Ap.....40..379M, 1998Ap.....41..161M, 1998Ap.....41..232M.
o	Table 1: <BIG NNNa> (Nos 180-238) N=89.
Ref:	=2001Ap.....44...33M
by	MICKAELIAN A.M.
	Astrophysics, 44, 33-45 (2001)
	Optical identifications of IRAS point sources. Galaxies. VI.
o	Table 1: <BIG NNNa> (Nos 239-298) N=87.
Ref:	=2001Ap.....44..185M
by	MICKAELIAN A.M.
	Astrophysics, 44, 185-198 (2001)
	Optical identifications of IRAS Point Sources. Galaxies. VII.
o	Table 1: <BIG NNNa> (Nos 299-361) N=95.
Ref:	=2002Ap.....45..288M
by	MICKAELIAN A.M.
	Astrophysics, 45, 288-301 (2002)
	Optical identifications of IRAS Point Sources. Galaxies. VIII.
o	Table 1: <BIG NNNa> (Nos 362-416) N=89.
Ref:	=2004Ap.....47...91M
by	MICKAELIAN A.M. , SARGSYAN L.A.
	Astrophysics, 47, 91-103 (2004)
	Optical identification of IRAS Point Sources Galaxies IX.
o	Table 1: <BIG NNNa> (Nos 417-476) N=87.
Ref:	=2004Ap.....47..213M
by	MICKAELIAN A.M. , SARGSYAN L.A.
	Astrophysics, 47, 213-228 (2004)
	Optical identification of IRAS point sources. Galaxies. X.
o	Table 1: <BIG NNNa> (Nos 476-536) N=104.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BIG2010]
[BIG2010]	(Bouwens+Illingworth+Gonzalez+, 2010)= (GNS)
Write:	<<[BIG2010] GNS-zDN>> <<[BIG2010] GNS-JDN>> <<[BIG2010] GNS-SpN>> <<[BIG2010] GNS-ON>>
N:	7+2+3+8
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	z850-, J-, spurious J- and other dropout galaxy candidates. Use of data from HST NICMOS+ACS observations over the two GOODS fields and the HDFS. Use of deep Subaru MOIRCS and VLT ISAAC ground-based data.
in source:	NAME HUDF
in source:	NAME GOODS South Field
in source:	NAME GOODS North Field
in source:	NAME HDFS
Ref:	=2010ApJ...725.1587B
by	BOUWENS R.J. , ILLINGWORTH G.D., GONZALEZ V., LABBE I., FRANX M., CONSELICE C.J., BLAKESLEE J., VAN DOKKUM P., HOLDEN B., MAGEE D., MARCHESINI D., ZHENG W.
	Astrophys. J., 725, 1587-1599 (2010)
	z ~ 7 galaxy candidates from NICMOS observations over the HDF-South and the CDF-South and HDF-North GOODS fields.
o	Table 2: <[BIG2010] GNS-zDN> (Nos GNS-zD1 to GNS-zD7), <[BIG2010] GNS-JDN> (Nos GNS-JD1 to GNS-JD2), <[BIG2010] GNS-SpN> (Nos GNS-Sp1 to GNS-Sp3), <[BIG2010] GNS-ON> (Nos GNS-ON1 to GNS-ON8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 1BIGB
1BIGB	(First Brazil ICRANet Gamma-ray Blazar)
Write:	<<1BIGB JHHMMSS.s+DDMMSS>>
N:	150
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	The first version of the Brazil ICRANet Gamma-ray Blazar catalog comprises N=150 gamma-ray excess signals detected out of 400 seed positions based on 2WHSP sources. See also 2BIGB.
Ref:	=2017A&A...598A.134A
by	ARSIOLI B. , CHANG Y.-L.
	Astron. Astrophys., 598A, 134-134 (2017)
	Searching for γ-ray signature in WHSP blazars. Fermi-LAT detection of 150 excess signal in the 0.3-500 GeV band.
o	Table A.1: <1BIGB JHHMMSS.s+DDMMSS> N=150.
=E=	Catalogue in electronic form as <J/A+A/598/A134/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 2BIGB
2BIGB	(Second Brazil-ICRANet Gamma-ray Blazars)
Write:	<<2BIGB JHHMMSS.s+DDMMSS>>
N:	1160
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	The Second Brazil-ICRANet Gamma-ray Blazar catalogue comprises N=1160 gamma-ray excess signatures detected out of 2013 seed positions based on 3HSP sources. Use of 3HSP and 4FGL data. See also 1BIGB.
Ref:	=2020MNRAS.493.2438A
by	ARSIOLI B. , CHANG Y.-L., MUSIIMENTA B.
	Mon. Not. R. Astron. Soc., 493, 2438-2451 (2020)
	Extreme and high synchrotron peak blazars beyond 4FGL: The 2BIGB γ-ray catalogue.
o	<2BIGB JHHMMSS.s+DDMMSS> N=1160.
=E=	Catalogue in electronic form as <J/MNRAS/493/2438/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BIH2008]
[BIH2008]	(Borissova+Ivanov+Hanson+, 2008)
Write:	<<[BIH2008] objNN>>
N:	10
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Las Companas Observatory 6.5m Baade telescopePANIC and VLT ISAAC observations of the star cluster [DBS2003] 179.
in source:	[DBS2003] 179
Ref:	=2008A&A...488..151B
by	BORISSOVA J. , IVANOV V.D., HANSON M.M., GEORGIEV L., MINNITI D., KURTEV R., GEISLER D.
	Astron. Astrophys., 488, 151-159 (2008)
	The young Galactic star cluster [DBS2003] 179.
o	Fig.2, Table 1: <[BIH2008] objNN> (Nos obj1-obj10).
Ref:	=2012A&A...546A.110B
by	BORISSOVA J. , GEORGIEV L., HANSON M.M., CLARKE J.R.A., KURTEV R., IVANOV V.D., PENALOZA F., HILLIER D.J., ZSARGO J.
	Astron. Astrophys., 546A, 110-110 (2012)
	Obscured clusters. IV. The most massive stars in [DBS2003] 179.
o	Tables 1: <[BIH2008] objNN> N=10 (Nos 11-20, 16 missing)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BII2011]
[BII2011]	(Biggs+Ivison+Ibar+, 2011)
Write:	<<[BII2011] VLA JHHMMSS.ssss+DDMMSS.sss>> <<[BII2011] MIPS JHHMMSS.ssss+DDMMSS.sss>> <<[BII2011] IRAC JHHMMSS.ssss+DDMMSS.sss>>
N:	100+148+39
Object:	(Rad) + (IR) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLA 1.4GHz and Spitzer MIPS (24µm) and IRAC (5.8µm) observations of N=126 LESS smm galaxies in the Extended Chandra Deep Field.
in source:	NAME ECDFS
Ref:	=2011MNRAS.413.2314B
by	BIGGS A.D. , IVISON R.J., IBAR E., WARDLOW J.L., DANNERBAUER H., SMAIL I., WALTER F., WEISS A., CHAPMAN S.C., COPPIN K.E.K., DE BREUCK C., DICKINSON M., KNUDSEN K.K., MAINIERI V., MENTEN K., PAPOVICH C.
	Mon. Not. R. Astron. Soc., 413, 2314-2338 (2011)
	The LABOCA survey of the Extended Chandra Deep Field-South – radio and mid-infrared counterparts to submillimetre galaxies.
o	Table 1: <[BII2011] VLA JHHMMSS.ssss+DDMMSS.sss> N=100. Table 2: <[BII2011] MIPS JHHMMSS.ssss+DDMMSS.sss> N=148. Table 3: <[BII2011] IRAC JHHMMSS.ssss+DDMMSS.sss> N=39.
=E=	Catalogue in electronic form as <J/MNRAS/413/2314/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BIL2011]
[BIL2011]	(Bouwens+Illengworth+Labbe+, 2011)
Write:	<<[BIL2011] UDFa-SSssMSSs>>
N:	7
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	J125- and Y105-dropout galaxies in the Hubble Ultra Deep Field. Format 'SSssMSSs': the complete J2000 coordinate format is 03 32 SS.ss (right ascension) and -27 4M SS.s (declination). Use of HST WFC3/IR data.
in source:	NAME HUDF
Ref:	=2011Natur.469..504B
by	BOUWENS R.J. , ILLINGWORTH G.D., LABBE I., OESCH P.A., TRENTI M., CAROLLO C.M., VAN DOKKUM P.G., FRANX M., STIAVELLI M., GONZALEZ V., MAGEE D., BRADLEY L.
	Natur, 469, 504-507 (2011)
	A candidate redshift z ~10 galaxy and rapid changes in that population at an age of 500 Myr.
o	Table 1: <[BIL2011] UDFa-SSssMSSs> (Nos UDFj-39546284, UDFy-38135539, UDFy-37796000, UDFy-33436598). Fig. S10: <[BIL2011] UDFj-SSssMSSs> (Nos UDFj-38116243, UDFj-35427336, UDFj-43696407).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BIL2018]
[BIL2018]	(Borissova+Ivanov+Lucas+, 2018)
Write:	<<[BIL2018] CLNNN ObjN>>
N:	5
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	ESO NTT SofI observations of N=3+2 stars in N=2 stellar cluster candidates (CLNNN in the format (VVVX).
in source:	VVVX CL10
in source:	VVVX CL11
Ref:	=2018MNRAS.481.3902B
by	BORISSOVA J. , IVANOV V.D., LUCAS P.W., KURTEV R., ALONSO-GARCIA J., RAMIREZ ALEGRIA S., MINNITI D., FROEBRICH D., HEMPEL M., MEDINA N., CHENE A.-N., KUHN M.A.
	Mon. Not. R. Astron. Soc., 481, 3902-3920 (2018)
	New Galactic star clusters discovered in the disc area of the VVVX survey.
o	Tables A1-B1: <VVVX CLNNN> (Nos CL1-CL120). Table 1: <[BIL2018] CLNNN ObjN> N=3+2 (Nos CL010 Obj1-CL010 Obj3, CL011 Obj1-CL011 Obj2)
=E=	Catalogue in electronic form as <J/MNRAS/481/3902/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BIMA
BIMA	(Berkeley-Illinois-Maryland Assoc.)
*****	Avoid the usage of BIMA, prefer [BGE2002]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BIO2010]
[BIO2010]	(Bouwens+Illingworth+Oesch+, 2010)
Write:	<<[BIO2010] UDFy-SSssMSSs>>
N:	5
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFC3 observations of z∼8-8.5 galaxies in the Hubble Ultra Deep Field. See also [OBI2010].
in source:	NAME HUDF
Ref:	=2010ApJ...709L.133B
by	BOUWENS R.J. , ILLINGWORTH G.D., OESCH P.A., STIAVELLI M., VAN DOKKUM P., TRENTI M., MAGEE D., LABBE I., FRANX M., CAROLLO C.M., GONZALEZ V.
	Astrophys. J., 709L, 133-137 (2010)
	Discovery of z ~ 8 galaxies in the Hubble ultra deep field from ultra-deep WFC3/IR observations.
o	Figs 1-3: <[BIO2010] UDFy-SSssMSSs> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BIO2011]
[BIO2011]	(Bouwens+Illingworth+Oesch+, 2011)
Write:	<<[BIO2011] UDFz-SSssMSSs>> <<[BIO2011] UDFy-SSssMSSs>> <<[BIO2011] UDF09Fa-SSssMSSs>> <<[BIO2011] ERSz-MSSssMMSSs>> <<[BIO2011] ERSY-MSSssMMSSs>>
N:	221
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Use of HST WFC3/IR and AVS available over HUDF09 and ERS (Early Release Science) fields to search for galaxies at z∼7 and z∼8. Format 'MSSssMMSSs': the complete 2000 coordinate format is 03 3M SS.ss (right ascension) and -27 MM SS.s (declination). See also [OBI2010], [BIG2010], [LBG2010].
in source:	NAME HUDF
Ref:	=2011ApJ...737...90B
by	BOUWENS R.J. , ILLINGWORTH G.D., OESCH P.A., LABBE I., TRENTI M., VAN DOKKUM P., FRANX M., STIAVELLI M., CAROLLO C.M., MAGEE D., GONZALEZ V.
	Astrophys. J., 737, 90 (2011)
	Ultraviolet luminosity functions from 132 z ~ 7 and z ~ 8 Lyman-break galaxies in the ultra-deep HUDF09 and wide-area Early Release Science WFC3/IR observations.
o	Tables 10+18: <[BIO2011] UDFz-SSssMSSs> N=29+7. Tables 11+12+15+16+18+19: <[BIO2011] UDF09Fa-SSssMSSs> N=17+14+14+16+21+30. Tables 13+20: <[BIO2011] ERSz-MSSssMSSs> N=13+23, <[BIO2011] ERSY-MSSssMSSs> N=6. Tables 14+19: <[BIO2011] UDFy-SSssMSSs> N=24+13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BIO2014]
[BIO2014]	(Bouwens+Illingworth+Oesch+, 2014)
Write:	<<[BIO2014] XDF-MSSssDMMSSs>>
N:	∼4000
Object:	G (SIMBAD class: Galaxy)
Note:	N∼4000 high-redshift galaxies (z∼4-8) from the HST HUDF/XDF, HUDF09-1, HUDF09-2, ERS, CANDELS-N and CANDELS-S data sets. Format 'MSSssDMMSSs': the complete 2000 coordinate format is 03 3M SS.ss (right ascension) and -2D MM SS.s (declination).
Ref:	=2014ApJ...793..115B
by	BOUWENS R.J. , ILLINGWORTH G.D., OESCH P.A., LABBE I., VAN DOKKUM P.G., TRENTI M., FRANX M., SMIT R., GONZALEZ V., MAGEE D.
	Astrophys. J., 793, 115 (2014)
	UV-continuum slopes of >4000 z ~ 4-8 galaxies from the HUDF/XDF, HUDF09, ERS, CANDELS-south, and CANDELS-north fields.
o	Tables 8-9: <[BIO2014] XDF-MSSssMMSSs> N~4000.
=E=	Catalogue in electronic form as <J/ApJ/793/115/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BIO2015]
[BIO2015]	(Bouwens+Illingworth+Oesch+, 2015)
Write:	<<[BIO2015] AAAA-NNNNNNNNNN>> <<[BIO2015] BORGY-NNNNNNNNNN>> <<[BIO2015] HUDF09NA-NNNNNNNNNN>> <<[BIO2015] AAAA-MSSssMMSSs>> (not recognised by Simbad, but found in literature) <<[BIO2015] BORGY-MSSssMMSSs>> <<[BIO2015] HUDF09NA-MSSssMMSSs>>
N:	10421
Object:	G (SIMBAD class: Galaxy)
Note:	N=10421 galaxy candidates at z≥4. Use of Hubble Space Telescope (HST) data sets from the CANDELS, HUDF09, HUDF12, ERS, and BoRG/HIPPIES programs.
Ref:	=2015ApJ...803...34B
by	BOUWENS R.J. , ILLINGWORTH G.D., OESCH P.A., TRENTI M., LABBE I., BRADLEY L., CAROLLO M., VAN DOKKUM P.G., GONZALEZ V., HOLWERDA B., FRANX M., SPITLER L., SMIT R., MAGEE D.
	Astrophys. J., 803, 34 (2015)
	UV luminosity functions at redshifts z ~ 4 to z ~ 10: 10,000 galaxies from HST legacy fields.
o	":" sign in data velocities = higher probability for being a lower-redshift.
o	Table 3: <[BIO2015] AAAA-NNNNNNNNNN>, <[BIO2015] BORGY-NNNNNNNNNN>, <[BIO2015] HUDF09NA-NNNNNNNNNN>, N=10421.
=E=	Catalogue in electronic form as <J/ApJ/803/34/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BIO2017]
[BIO2017]	(Bouwens+Illingworth+Oesch+, 2017)
Write:	<<[BIO2017] {A2744}{I\|U\|V\|Y\|Z}-MSSssMMSSs>> <<[BIO2017] {M0416\|M0717\|M1149}{I\|U\|V\|Y\|Z}-MSSssMMSSs>>
N:	236
Object:	Grav. lensed image of a G (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFC3 NIR observations of N=232 faint galaxies lensed by N=4 of the Hubble Frontier Fields (HFF) clusters at 2<z<8. See also [BIO2015] and [LFL2017].
in source:	ACO 2744
in source:	MCS J0416.1-2403
in source:	ClG J0717+3745 = MCS J0717.5+3745
in source:	MCS J1149.6+2223
Ref:	=2017ApJ...843...41B
by	BOUWENS R.J. , ILLINGWORTH G.D., OESCH P.A., ATEK H., LAM D., STEFANON M.
	Astrophys. J., 843, 41-41 (2017)
	Extremely small sizes for faint z ~ 2-8 galaxies in the Hubble Frontier Fields: a key input for establishing their volume density and UV emissivity.
o	[BIO2017] M0416I-6122135929 is not in Simbad because not in the good format.
o	Table 2: <[BIO2017] A2744A-MSSssMMSSs> N=60, <[BIO2017] M0416A-MSSssMMSSs> N=57, <[BIO2017] M0717A-MSSssMMSSs> N=70, <[BIO2017] M1149A-MSSssMMSSs> N=49.
=E=	Catalogue in electronic form as J/ApJ/843/41
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Bip
Bip	(Bipolar neb.)
*****	Avoid the usage of Bip, prefer [NS84]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BIP2021]
[BIP2021]	(Benaglia+Ishwara-Chandra+Paredes+, 2021)
Write:	<<[BIP2021] SNN>>
N:	47
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	GMRT 325 and 610MHz observations of N=47 radio sources in the field of gamma-ray sources in the Cygnus region.
in source:	NAME Cygnus Region
Ref:	=2021ApJS..252...17B
by	BENAGLIA P. , ISHWARA-CHANDRA C.H., PAREDES J.M., INTEMA H.T., COLAZO M.E., ISEQUILLA N.L.
	Astrophys. J., Suppl. Ser., 252, 17-17 (2021)
	Radio counterparts of γ-ray sources in the Cygnus Region.
o	Figs 3-15, Tables 3-4: <[BIP2021] SNN> (Nos S1-S47).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BIR2003]
[BIR2003]	(Bouwens+Illingworth+Rosati+, 2003)
Write:	<<[BIR2003] J1252-NNNN-NNNN>> <<[BIR2003] HDF-N NNNN-NNNN>>
N:	21+2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ISAAC data for the RDCS J1252-2927 field and NICMOS data for the HDF-N field: sample of of galaxies with z about 6.
in source:	RDCS J1252-2927
in source:	NAME HDFN
Ref:	=2003ApJ...595..589B
by	BOUWENS R.J. , ILLINGWORTH G.D., ROSATI P., LIDMAN C., BROADHURST T., FRANX M., FORD H.C., MAGEE D., BENITEZ N., BLAKESLEE J.P., MEURER G.R., CLAMPIN M., HARTIG G.F., ARDILA D.R., BARTKO F., BROWN R.A., BURROWS C.J., CHENG E.S., CROSS N.J.G., FELDMAN P.D., GOLIMOWSKI D.A., GRONWALL C., INFANTE L., KIMBLE R.A., KRIST J.E., LESSER M.P., MARTEL A.R., MENANTEAU F., MILEY G.K., POSTMAN M., SIRIANNI M., SPARKS W.B., TRAN H.D., TSVETANOV Z.I., WHITE R.L., ZHENG W.
	Astrophys. J., 595, 589-602 (2003)
	Star formation at z~6: i-dropouts in the Advanced Camera for Surveys Guaranteed Time Observation fields.
o	Table 1: <[BIR2003] J1252-NNNN-NNNN> N=21, <[BIR2003] HDF-N NNNN-NNNN> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BIR96]
[BIR96]	(Brandt+Iwasawa+Reynolds, 1996) (Not yet in Simbad)
Write:	<<[BIR96] NGC 4945 X-1>>
N:	1
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT PSPC observations of N=1 variable X-ray source in NGC 4945.
in source:	NGC 4945
Ref:	=1996MNRAS.281L..41B
by	BRANDT W.N. , IWASAWA K., REYNOLDS C.S.
	Mon. Not. R. Astron. Soc., 281, 41-45 (1996)
	A powerful and higly variable off-nuclear X-ray source in the composite starburst/Seyfert 2 galaxy NGC 4945.
o	<[BIR96] NGC 4945 X-1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BIRS
BIRS	(Bright Infrared *)
Write:	<<BIRS NNN>>
N:	137
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	2deg x3deg surveyed near W 3, W 4
Ref:	=1980ApJ...240..846E
by	ELMEGREEN D.M.
	Astrophys. J., 240, 846-852 (1980)
	Star formation in W3 and W4: discovery of 135 possibly embedded near-infrared stars.
o	Table 1: <BIRS NNN> (Nos 1-137)
Details on Acronym: BIS
BIS	(Byurakan, IR Star)
Write:	<<BIS NNN>>
N:	275
Object:	* (SIMBAD class: Star)
Note:	FBS IRAS stars. Stars and galaxies are simultaneously included in the 1st ref., and a general numbering was made. See [M97c], BIG. 2000Ap.....43...55M: They were 61 and 76 stars in the first two published lists (refs 1997Ap.....40....1M and 1999Ap.....42...37G), so the stars in the present list are numbered starting with 138. THe catalogue of BIS stars is revised and updated in 2006A&A...455..765M.
Ref:	=1997Ap.....40....1M
by	MICKAELIAN A.M.
	Astrophysics, 40, 1-9 (1997)
	Optical identification of 100 IRAS point sources at high galactic latitude.
o	Galaxies 'BIG NN' and stars 'BIS NN' are not numbered here, they are respectively the galaxies and the stars included in [M97c] NNN objects.
o	Table 1: <[M97c] NNN> (Nos 1-100). Table 1: <BIG NN> N=? Table 1: <BIS NN> (Nos 1-61)?
Ref:	=1999Ap.....42...37G
by	GIGOYAN K.S. , MICKAELIAN A.M.
	Astrophysics, 42, 37-42 (1999)
	Optical identification of IRAS point sources based on low-dispersion spectra from the First Byurakan Survey. V.
o	Stars 'BIS NNN' are not numbered here, they are added to the stars in the first '[M97c]' reference: 1997Ap.....40....1M.
o	Table 1: <[M97c] NNN> N=19 among (Nos 242-315). Table 1: <BIS NNN> (Nos 62-137)?
Ref:	=2000Ap.....43...55M
by	MICKAELIAN A.M. , GIGOYAN K.S.
	Astrophysics, 43, 55-61 (2000)
	Optical identification of IRAS point sources based on low-dispersion FBS spectra. Stars. III.
o	BIS numbering (Nos 1-137) are the stars in 1997Ap.....40....1M, 1999Ap.....42...37G; in ref list IYENGAR instead of LYENG AR
o	Table 1: <BIS NNN> (Nos 138-171).
Ref:	=2000Ap.....43..262G
by	GIGOYAN K.S. , MICKAELIAN A.M.
	Astrophysics, 43, 262-268 (2000)
	Optical identification of IRAS point sources based on low-dispersion FBS spectra. Stars. IV.
o	Table 1: <BIS NNN> (Nos 172-212).
Ref:	=2001Ap.....44..222M
by	MICKAELIAN A.M. , GIGOYAN K.S.
	Astrophysics, 44, 222-232 (2001)
	Optical identification of IRAS point sources based on low-dispersion FBS spectra. Stars. V.
o	Table 1: <BIS NNN> (Nos 213-287).
Ref:	=2006A&A...455..765M
by	MICKAELIAN A.M. , GIGOYAN K.S.
	Astron. Astrophys., 455, 765-772 (2006)
	Revised and updated catalogue of Byurakan-IRAS stars.
o	Catalogue: <BIS NNN> N=276 among (Nos 1-287).
=E=	Catalogue in electronic form as III/237
=E=	Catalogue in electronic form as J/A+A/455/765
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BIS2007]
[BIS2007]	(Borissova+Ivanov+Stephens+, 2007)
Write:	<<[BIS2007] JHHMMSS.ss+DDMMSS.ss>> <<[BIS2007] VN>> <<[BIS2007] xxx.xx-yy.yyy>>
N:	15+5+2142
Object:	* in Cl* (SIMBAD class: Star)
Note:	VLT ISAAC NIR spectroscopy of the globular cluster [HJK2000] GC02.
in source:	[HJK2000] GC02
Ref:	=2007A&A...474..121B
by	BORISSOVA J. , IVANOV V.D., STEPHENS A.W., CATELAN M., MINNITI D., PRIETO G.
	Astron. Astrophys., 474, 121-127 (2007)
	A deep near-infrared view of the Galactic globular cluster 2MASS GC02.
o	Table 1: <[BIS2007] JHHMMSS.ss+DDMMSS.ss> N=15. Table 3: <[BIS2007] VN> (Nos V1-V5). Catalog: <[BIS2007] xxx.xx-yy.yyy> N=2142.
=E=	Catalogue in electronic form as J/A+A/474/121
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BIT2005]
[BIT2005]	(Bouwens+Illingworth+Thompson+, 2005)= (HDFN) = (HDFSPAR) = (UDF) = (UDFNICPAR1) = (UDFNICPAR2)
Write:	<<[BIT2005] UDFNICPAR1 SSssMSSs>> <<[BIT2005] UDFNICPAR2 SSssMSSs>> <<[BIT2005] UDF SSssMSSs>> <<[BIT2005] HDFN SSssMSSs>> <<[BIT2005] HDFSPAR SSssMSSs>>
N:	11
Object:	G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Search for red objects in the NICMOS-ACS parallel fields. In the second part of the format (SSssMSSs), the 4 first SSss stands for the last four significant digits of right ascension, the 4 last MSSs for the last four significant digits of Declination.
in source:	NAME HUDF
in source:	NAME HDFN
in source:	NAME HDFS
Ref:	=2005ApJ...624L...5B
by	BOUWENS R.J. , ILLINGWORTH G.D., THOMPSON R.I., FRANX M.
	Astrophys. J., 624, 5-8 (2005)
	Constraints on z~10 galaxies from the deepest Hubble Space Telescope NICMOS fields.
o	Table 2: <[BIT2005] UDFNICPAR1 SSssMSSs> N=3, <[BIT2005] UDFNICPAR2 SSssMSSs> N=2, <[BIT2005] UDF SSssMSSs> N=2, <[BIT2005] HDFN SSssMSSs> N=3, <[BIT2005] HDFSPAR SSssMSSs> N=1.
=E=	Catalogue in electronic form as J/ApJ/624/L5
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Biur
Biur	(Biurakan obs.)
*****	Avoid the usage of Biur, prefer Biurakan
Details on Acronym: Biurakan
Biurakan	(Biurakan obs.)= (Biur) = (Bjurakan)
Write:	<<Cl Biurakan NN>>
N:	13
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Details on Acronym: [BIW2023]
[BIW2023]	(Booth+Ilee+Walsh+, 2023)
Write:	<<[BIW2023] J173.360-70.193>>
N:	1
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 7 observations of N=1 sub-millimeter source near HD 100546.
Ref:	=2023A&A...669A..53B
by	BOOTH A.S. , ILEE J.D., WALSH C., KAMA M., KEYTE L., VAN DISHOECK E.F., NOMURA H.
	Astron. Astrophys., 669A, 53 (2023)
	Sulphur monoxide emission tracing an embedded planet in the HD 100546 protoplanetary disk.
o	Fig. C.1: <[BIW2023] J173.360-70.193> N=1.
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [BJ84]
[BJ84]	(Benson+Johnston, 1984)= (Sgr) = (Sgr B2)
Write:	<<[BJ84] A>> <<[BJ84] AN>> <<[BJ84] AA>> <<[BJ84] ANa>>
N:	37+18+1
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	(Nos A-Z, M,N,S missing), (Nos A1-A2, F1-F4, K1-K6), (Nos AA, BB), N=18 (Nos FNa). Nos M, N, S are excluded: The designations Sgr B2 (M), Sgr B2 (N) and Sgr B2 (S) correspond to regions (Main), (North) and (South), not HII regions. In SIMBAD they are designated as 'NAME Sgr B2 (M)', (N) and (S). NAME Sgr B2 (M) = [BJ84] A to G + J + Y + Z NAME Sgr B2 (N) = [BJ84] K NAME Sgr B2 (S) = [BJ84] H In ref. 1998ApJ...500..847D, the regions F1-F4 are subdivised in several components 'FNa' See also [GCD95]
in source:	NAME Sgr B2
Ref:	=1984ApJ...277..181B
by	BENSON J.M. , JOHNSTON K.J.
	Astrophys. J., 277, 181-188 (1984)
	Arc second resolution maps of the compact sources in Sagittarius B2 and G 34.3+0.2.
o	<[BJ84] A> (Nos A-L)
Ref:	=1990ApJ...351..538G
by	GAUME R.A. , CLAUSSEN M.J.
	Astrophys. J., 351, 538-562 (1990)
	The Sagittarius B2 star-forming region: subarcsecond radio spectral line and continuum observations.
o	<[BJ84] AN> (Nos A1-A2, F1-F4, K1-K5).
Ref:	=1993ApJ...412..684M
by	MEHRINGER D.M. , PALMER P., GOSS W.M., YUSEF-ZADEH F.
	Astrophys. J., 412, 684-695 (1993)
	Radio continuum and radio recombination line observations of Sagittarius B2.
o	<[BJ84] A> (Nos O-Z, M,N,S missing). <[BJ84] AA> (Nos AA, BB). <[OF84] NNA> (Nos 35A, 35B, 35C) added.
Ref:	=1995ApJ...449..663G
by	GAUME R.A. , CLAUSSEN M.J., DE PREE C.G., GOSS W.M., MEHRINGER D.M.
	Astrophys. J., 449, 663-673 (1995)
	The Sagittarius B2 star-forming region. I. Sensitive 1.3 centimeter continuum observations.
o	Table 2: <[BJ84] K6> N=1 added. Table 2: <[GCD95] ASS.ss> N=23
Ref:	=1998ApJ...500..847D
by	DE PREE C.G. , GOSS W.M., GAUME R.A.
	Astrophys. J., 500, 847-852 (1998)
	Ionized gas in Sagittarius B2 main on scales of 0.065 arcsecond (600 AU).
o	Table 1: <[GCD95] F10.38> N=1 added. Table 1: <[BJ84] FNa> (Nos F1a-F1g, F2a-F2d, F3a-F3e, F4a-F4c).
Ref:	=2015ApJ...815..123D
by	DE PREE C.G. , PETERS T., MAC LOW M.M., WILNER D.J., GOSS W.M., GALVAN-MADRID R., KETO E.R., KLESSEN R.S., MONSRUD A.
	Astrophys. J., 815, 123 (2015)
	Evidence of short timescale flux density variations of UC HII regions in Sgr B2 Main and North.
o	Tables 3: <[BJ84] K7> N=1 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BJ92]
[BJ92]	(Bhatt+Jain, 1992)
Write:	<<[BJ92] NN>>
N:	19
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	MBM 12
Ref:	=1992MNRAS.257...57B
by	BHATT H.C. , JAIN S.K.
	Mon. Not. R. Astron. Soc., 257, 57-61 (1992)
	Polarization measurements of stars in the region of the nearby molecular cloud MBM 12.
o	<[BJ92] NN> N=19
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BJ93]
[BJ93]	(Bhatt+Jain, 1993)
Write:	<<[BJ93] B 227 NN>> <<[BJ93] L 121 NN>>
N:	21+12
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 1: format 'B 227 NN', N=21 * in the region of Barn 227 Table 2: format 'L 121 NN', N=12 * in the region of LDN 121
in source:	Barnard 227
in source:	LDN 121
Ref:	=1993A&A...276..507B
by	BHATT H.C. , JAIN S.K.
	Astron. Astrophys., 276, 507-510 (1993)
	Polarization maps for the dark clouds B 227 and L 121.
o	Table 1: <[BJ93] B 227 NN> N=21, Table 2: <[BJ93] L 121 NN> N=12
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BJB2016]
[BJB2016]	(Bihr+Johnston+Beuther+, 2016)
Write:	<<[BJB2016] GLLL.lll+BB.bbb>> <<[BJB2016] G032.875-00.420A>> <<[BJB2016] G032.875-00.420B>>
N:	10387
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA observations from 1 to 2GHz of N=10387 Galactic continuum sources, as part of the HI, OH, Recombination line (THOR) survey. Two sources have the same Galactic identifier in the catalog, therefore the CDS added a suffix A and B to differentiate them in SIMBAD.
Ref:	=2016A&A...588A..97B
by	BIHR S. , JOHNSTON K.G., BEUTHER H., ANDERSON L.D., OTT J., RUGEL M., BIGIEL F., BRUNTHALER A., GLOVER S.C.O., HENNING T., HEYER M.H., KLESSEN R.S., LINZ H., LONGMORE S.N., McCLURE-GRIFFITHS N.M., MENTEN K.M., PLUME R., SCHIERHUBER T., SHANAHAN R., STIL J.M., URQUHART J.S., WALSH A.J.
	Astron. Astrophys., 588A, 97-97 (2016)
	Continuum sources from the THOR survey between 1 and 2 GHz.
o	Catalog: <[BJB2016] GLLL.lll+BB.bbb> N=4420, <[BJB2016] G032.875-00.420A> (Nos A-B).
Ref:	=2018A&A...619A.124W
by	WANG Y. , BIHR S., RUGEL M., BEUTHER H., JOHNSTON K.G., OTT J., SOLER J.D., BRUNTHALER A., ANDERSON L.D., URQUHART J.S., KLESSEN R.S., LINZ H., McCLURE-GRIFFITHS N.M., GLOVER S.C.O., MENTEN K.M., BIGIEL F., HOARE M., LONGMORE S.N.
	Astron. Astrophys., 619A, 124-124 (2018)
	Radio continuum emission in the northern Galactic plane: Sources and spectral indices from the THOR survey.
o	(Erratum) erratum vol. 641, art. C1 (2020)
o	Catalog: <[BJB2016] GLLL.lll+BB.bbb> N=10387.
=E=	Catalogue in electronic form as <J/A+A/588/A97/>
=E=	Catalogue in electronic form as <J/A+A/619/A124/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BJD2020]
[BJD2020]	(Bowler+Jarvis+Dunlop+, 2020)
Write:	<<[BJD2020] XMMN-NNNN>> <<[BJD2020] UDS-NNN>> <<[BJD2020] UVISTA-NNNN>>
N:	6+6+16
Object:	Poss. LBG (SIMBAD class: Galaxy)
Note:	N=28 high-redshift Lyman break galaxy (LBG) candidates in the COSMOS and the XMM-Newton Large-Scale Structure (XMM-LSS) fields. Use of UltraVISTA DR4, VIDEO, and UKIRT UDS near-infrared data.
in source:	NAME COSMOS Field
in source:	NAME XMM-LSS Field
Ref:	=2020MNRAS.493.2059B
by	BOWLER R.A.A. , JARVIS M.J., DUNLOP J.S., McLURE R.J., McLEOD D.J., ADAMS N.J., MILVANG-JENSEN B., McCRACKEN H.J.
	Mon. Not. R. Astron. Soc., 493, 2059-2084 (2020)
	A lack of evolution in the very bright end of the galaxy luminosity function from z ≃ 8 to 10.
o	Tables 3-4: <[BJD2020] XMMN-NNNN> (Nos XMM1-994, XMM2-3904, XMM2-4314, XMM3-3085, XMM3-5645, XMM3-6787), <[BJD2020] UDS-NNN> N=6 among (Nos 74-787), <[BJD2020] UVISTA-NNNN> N=16 among (Nos 213-1212).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BJE84]
[BJE84]	(Beichman+Jennings+Emerson+, 1995)= (IRS)
Write:	<<[BJE84] IRS N>>
N:	4
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	IRAS observations
in source:	Barnard 5
Ref:	=1984ApJ...278L..45B
by	BEICHMAN C.A. , JENNINGS R.E., EMERSON J.P., BAUD B., HARRIS S., ROWAN-ROBINSON M., AUMANN H.H., GAUTIER T.N., GILLETT F.C., HABING H.J., MARSDEN P.L., NEUGEBAUER G., YOUNG E.
	Astrophys. J., 278, 45-48 (1984)
	The formation of solar type stars : IRAS observations of the dark cloud Barnard 5.
o	Table 1: <[BJE84] IRS N> (Nos 1-4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BJF
BJF	(Brocksopp+Jonker+Fender+)
Write:	<<BJF JHHMMSS.ss+DDMMSS.s>>
N:	8
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=8 reference stars in the field of BW Cir.
Ref:	=2001MNRAS.323..517B
by	BROCKSOPP C. , JONKER P.G., FENDER R.P., GROOT P.J., VAN DER KLIS M., TINGAY S.J.
	Mon. Not. R. Astron. Soc., 323, 517-528 (2001)
	The 1997 hard-state outburst of the X-ray transient GS 1354-64/BW Cir.
o	Table 2: <BJF JHHMMSS.ss+DDMMSS.s> N=8.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BJF2004]
[BJF2004]	(Biller+Jones+Forman+, 2004)
Write:	<<[BJF2004] JHHMMSS.sss+DDMMSS.ss>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS observations of two extended sources in NGC 4472.
in source:	NGC 4472
Ref:	=2004ApJ...613..238B
by	BILLER B.A. , JONES C., FORMAN W.R., KRAFT R., ENSSLIN T.
	Astrophys. J., 613, 238-246 (2004)
	Hot gas structure in the elliptical galaxy NGC 4472.
o	Table 2: <[BJF2004] JHHMMSS.sss+DDMMSS.ss> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BJG2004]
[BJG2004]	(Balaguer-Nunez+Jordi+Galadi-Enriquez+, 2004)
Write:	<<[BJG2004] NNNN>>
N:	7842
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Observations from Calar Alto and ORM La Palma. Deep CCD photometry of the area of NGC 1817 and NGC 1807.
in source:	NGC 1817
in source:	NGC 1807
Ref:	=2004A&A...426..827B
by	BALAGUER-NUNEZ L. , JORDI C., GALADI-ENRIQUEZ D., MASANA E.
	Astron. Astrophys., 426, 827-834 (2004)
	uvby-H_{β} CCD photometry of NGC 1817 and NGC 1807.
o	Table 4: <[BJG2004] NNNN> (Nos 1-7842).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BJG2014]
[BJG2014]	(Bayliss+Johnson+Gladders+, 2014)
Write:	<<[BJG2014] JHHMMSS.s+DDMMSSa>>
N:	2221
Object:	G (SIMBAD class: Galaxy)
Note:	MMT Hectospec, Magellan IMACS, and Gemini GMOS-N spectroscopy of N=2221 galaxies in nine galaxy clusters.
Ref:	=2014ApJ...783...41B
by	BAYLISS M.B. , JOHNSON T., GLADDERS M.D., SHARON K., OGURI M.
	Astrophys. J., 783, 41 (2014)
	Line-of-sight structure toward strong lensing galaxy clusters.
o	Table 2: <[BJG2014] JHHMMSS.s+DDMMSSa> N=2221.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BJH2016]
[BJH2016]	(Brown+Johnston+Hoare+, 2016)
Write:	<<[BJH2016] VLA N>>
N:	7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 5GHz, 8.5GHz, and 22.5GHz continuum observations of N=7 radio sources in the field of IRAS 05373+2349.
Ref:	=2016MNRAS.463.2839B
by	BROWN G.M. , JOHNSTON K.G., HOARE M.G., LUMSDEN S.L.
	Mon. Not. R. Astron. Soc., 463, 2839-2848 (2016)
	Connecting low- and high-mass star formation: the intermediate-mass protostar IRAS 05373+2349 VLA 2.
o	Table 3: <[BJH2016] VLA N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BJI2000]
[BJI2000]	(Bolatto+Jackson+Israel+, 2000)
Write:	<<[BJI2000] RN>> <<[BJI2000] N159 R>> <<[BJI2000] N160 R>>
N:	2+3+3
Object:	Region + (Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=2 regions, (Nos R1-R2), with low-level extended emission in 12CO in LHA 120-N 159 + LHA 120-N 160 complex. N=3 radio continuum sources in LHA 120-N 159 and N=3 radio continuum sources in LHA 120-N 160.
in source:	Magellanic Clouds:LMC:LHA 120-N 159 = LHA 120-N 159
in source:	Magellanic Clouds:LMC:LHA 120-N 160 = LHA 120-N 160
Ref:	=2000ApJ...545..234B
by	BOLATTO A.D. , JACKSON J.M., ISRAEL F.P., ZHANG X., KIM S.
	Astrophys. J., 545, 234-250 (2000)
	Carbon in the N159/N160 complex of the Large Magellanic Cloud.
o	Table 1: <[BJI2000] AN> (Nos R1-R2). Table 5: <[BJI2000] N159 R> (Nos I to III), <[BJI2000] N160 R> (Nos I to III).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BJI2006]
[BJI2006]	(Bassa+Jonker+In't Zand+, 2006)
Write:	<<[BJI2006] Star A>> <<[BJI2006] Single Star>>
N:	3
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Optical counterparts of 1A 1246-588 (Star X) and 4U 1812-12 (Single Star). Star A is another blue star in the field of 1A 1246-588.
Ref:	=2006A&A...446L..17B
by	BASSA C.G. , JONKER P.G., IN'T ZAND J.J.M., VERBUNT F.
	Astron. Astrophys., 446, 17-20 (2006)
	Two new candidate ultra-compact X-ray binaries.
o	Fig.1, text: <[BJI2006] Star A> (Nos A, X), <[BJI2006] Single Star> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BJJ2001]
[BJJ2001]	(Bowen+Jimenez+Jenkins+, 2001)
Write:	<<[BJJ2001] NNNN>>
N:	65
Object:	G (SIMBAD class: Galaxy)
Note:	N=65 galaxies close to the sight line of QSO 2302+029.
Ref:	=2001ApJ...547...39B
by	BOWEN D.V. , JIMENEZ R., JENKINS E.B., PETTINI M.
	Astrophys. J., 547, 39-49 (2001)
	Where are the absorbers toward Q2302+029?
o	Tables 1, 3: <[BJJ2001] NNNN> N=41+24 among (Nos 65-1000).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BJJ2001b]
[BJJ2001b]	(Bally+Jojnstone+Joncas+, 2001) (Not yet in Simbad)
Write:	<<[BJJ2001b] HH 559 Knot N>> <<[BJJ2001b] LL Ori 6 A>>
N:	3+9
Object:	Feature (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	See also [BOM2000] and [BR2001].
in source:	NAME Orion Nebula
Ref:	=2001AJ....122.1508B
by	BALLY J. , JOHNSTONE D., JONCAS G., REIPURTH B., MALLEN-ORNELAS G.
	Astron. J., 122, 1508-1524 (2001)
	Kinematics of optical outflows in the Orion nebula. I. The giant outflow HH 400 and the irradiated jet HH 502.
o	Table 3: <[BJJ2001b] HH 559 Knot N> (Nos 1-3), <[BJJ2001b] LL Ori 6 A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BJK80]
[BJK80]	(Burbidge+Junkkarinen+Koski+, 1980)
Write:	<<[BJK80] N>>
N:	6
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	QSO in the vicinity of M 82 [BJK80] 1 to 3 are known as HOAG 1 to 3 (NAME Hoag in SIMBAD)
Ref:	=1980ApJ...242L..55B
by	BURBIDGE E.M. , JUNKKARINEN V.T., KOSKI A.T., SMITH H.E., HOAG A.A.
	Astrophys. J., 242, 55-57 (1980)
	A "cluster" of Quasi-Stellar Objects near M 82.
o	<NAME HOAG N> = <[BJK80] N> (Nos 1-3)
Ref:	=1983ApJ...271..479A
by	ARP H.
	Astrophys. J., 271, 479-506 (1983)
	Further observations and analysis of quasars near companion galaxies.
o	Companions galaxies are not in SIMBAD.
o	Tables 5,6: [A83] use <[A81b] NGC NNNN UB NN> N=18 new. Table 5, Fig.7: <[BJK80] N> No. 4 is new
Ref:	=1989AN....310..187B
by	BOLLER T. , LORENZ H., AFANAS'EV V.L., DODONOV S.N., TEREBIZH V.Y.
	Astron. Nachr., 310, 187-193 (1989)
	On the cosmological evolution of the quasar population.
o	Table 4: <Boller NNN> N=6 among 254. Fig.2: <[BJK80] N> Nos 5, 6 are new
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BJL2004]
[BJL2004]	(Bremer+Jensen+Lehnert+, 2004) (Not yet in Simbad)
Write:	<<[BJL2004] N>>
N:	4
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Gemini data of the field of [PSR2004] 1916, a candidate z=10 galaxy in the foreground field of the cluster ACO 1835. 4 other objects are found in the field.
in source:	ACO 1835
Ref:	=2004ApJ...615L...1B
by	BREMER M.N. , JENSEN J.B., LEHNERT M.D., FOERSTER-SCHREIBER N.M., DOUGLAS L.
	Astrophys. J., 615, 1-4 (2004)
	Gemini H-band imaging of the field of a z = 10 candidate.
o	Table 1, Fig.2: Galaxy Candidate = [PSR2004] 1916.
o	Table 1, Fig.2: <[BJL2004] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BJM
BJM	(Baart+de Jager+Mountfort)= (BDM)
Write:	<<BJM NN>>
N:	20
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
in source:	Ass Sco OB 2
Ref:	=1980A&A....92..156B
by	BAART E.E. , DE JAGER G., MOUNTFORT P.I.
	Astron. Astrophys., 92, 156-162 (1980)
	A 2.3 GHz radio continuum map of the Upper Scorpio region.
o	<BJM NN> N=20
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BJR86]
[BJR86]	(Bahcall+Jones+Ratnatunga, 1986)
Write:	<<[BJR86] NNa>> <<[BJR86] BNa>>
N:	72+14
Object:	* in ** (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 1A: N=36x2 stars in pair, format 'NNa' Table 1B: N=7x2 stars in pair, format 'BNa' We don't use the format in col.(2), which will be ambiguous (same format for [BJR86] 9 and [BJR86] 30 for ex.)
Ref:	=1986ApJS...60..939B
by	BAHCALL J.N. , JONES B.F., RATNATUNGA K.U.
	Astrophys. J., Suppl. Ser., 60, 939-943 (1986)
	Wide binaries in the direction of Andromeda.
o	Table 1A: <[BJR86] NNa> N=36x2, Table 1B: <[BJR86] BNa> N=7x2
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BJS91]
[BJS91]	(Boyle+Jones+Shanks, 1991)
Write:	<<[BJS91] F855:NNN>> <<[BJS91] F861:NNN>> <<[BJS91] F864:NNN>>
N:	234+196+197
Object:	QSO + Faint Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Ref:	=1991MNRAS.251..482B
by	BOYLE B.J. , JONES L.R., SHANKS T.
	Mon. Not. R. Astron. Soc., 251, 482-507 (1991)
	A spectroscopic survey of faint QSOs.
o	Tables 6, 9: <[BJS91] AFFF:NNN> N=236
=E=	Catalogue in electronic form as J/MNRAS/251/482
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BJS99]
[BJS99]	(Budding+Jones+Slee+, 1999)
Write:	<<[BJS99] N>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA observations. N=3 radio-sources in the field of CF Tuc See also [GMD97]
Ref:	=1999MNRAS.305..966B
by	BUDDING E. , JONES K.L., SLEE O.B., WATSON L.
	Mon. Not. R. Astron. Soc., 305, 966-976 (1999)
	Coordinated multiwavelength observations of the RS CVn system CF Tuc.
o	Table 2: <[BJS99] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Bjurakan
Bjurakan	(Biurakan obs.)
*****	Avoid the usage of Bjurakan, prefer Biurakan
Details on Acronym: BK
BK	(Borngen+Karchentseva)= (BoKar)
Write:	<<BK NN>>
N:	8
Object:	Dwarf G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	in M81/82 group. Identif. charts. (BK1N to BK8N) In the format, the letter 'N' stands for New and objects are often found in the literature with this format. See also BK85 in IC 342 group
in source:	NAME M 81 GROUP
Ref:	=1982AN....303..189B
by	BORNGEN F. , KARACHENTSEVA V.E.
	Astron. Nachr., 303, 189-192 (1982)
	New dwarf galaxies in M 81/ M 82 group.
o	<BK1N> to <BK8N> N=8
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BK
BK	(Borngen+Karchentseva)
*****	Avoid the usage of BK, prefer BK85
Origin	of the Acronym: L (1997A&A...322..375H)
Details on Acronym: [BK2002]
[BK2002]	(Bresolin+Kennicutt, 2002)
Write:	<<[BK2002] M 83 NN>> <<[BK2002] M 83 A>> <<[BK2002] NGC 3351 N>> <<[BK2002] NGC 3351 A>> <<[BK2002] NGC 6384 N>>
N:	16+6+3
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	EFOSC2 ESO 3.6m telescope observations. Sample of extragalactic HII regions format 'NN' in 3 spiral galaxies, among them some are hot spots format 'A'.
in source:	M 83 = NGC 5236
in source:	NGC 3351
in source:	NGC 6384
Ref:	=2002ApJ...572..838B
by	BRESOLIN F. , KENNICUTT R.C.Jr
	Astrophys. J., 572, 838-860 (2002)
	Optical spectroscopy of metal-rich H II regions and circumnuclear hot spots in M83 and NGC 3351.
o	In reflist, Rumstay and al., 1983 : page 64 is a misprint for 611 (1983ApJ.274.611R).
o	Table 1: <[BK2002] M 83 NN> (Nos 1-11), <[BK2002] M 83 A> (Nos A-E), <[BK2002] NGC 3351 N> (Nos 1-2), <[BK2002] NGC 3351 A> (Nos A-D), <[BK2002] NGC 6384 N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BK2004]
[BK2004]	(Blaszkiewicz+Kus, 2004)
Write:	<<[BK2004] JHHMMSS.s+DDMMSS>>
N:	50
Object:	CH3OH Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	Torun radio telescope observations. Results of a methanol survey towards star forming sources containg 6.7 GHz maser emission sources.
Ref:	=2004A&A...413..233B
by	BLASZKIEWICZ L. , KUS A.J.
	Astron. Astrophys., 413, 233-240 (2004)
	12.2GHz survey towards 6.7GHz methanol masers. A comparison of 12.2GHz and 6.7GHz spectra.
o	Tables 2, 3: 22543+6139 is a misprint for IRAS 22543+6145 (found by coordinates)
o	Tables 2, 3: <[BK2004] JHHMMSS.s+DDMMSS> N=50.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BK2011]
[BK2011]	(Bhalerao+Kulkarni, 2011)
Write:	<<[BK2011] A>>
N:	11
Object:	* (SIMBAD class: Star)
Note:	Keck LRIS observations of the field of PSR J1614-2230.
Ref:	=2011ApJ...737L...1B
by	BHALERAO V.B. , KULKARNI S.R.
	Astrophys. J., 737L, 1 (2011)
	The white dwarf companion of a 2 m☉ neutron star.
o	Fig. 1, Table 1: <[BK2011] A> N=11 among (Nos A-S).
o	In fig.3: M15 C is not identified.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BK2016]
[BK2016]	(Belokurov+Koposov, 2016)
Write:	<<[BK2016] SN>>
Object:	Stellar Stream + Stellar Cloud (SIMBAD class: Association = Association of Stars)
Stat:	is completely incorporated in Simbad
Note:	N=4 Magellanic stellar halo structures. Use of Dark Energy Survey (DES) Year 1 public data.
Ref:	=2016MNRAS.456..602B
by	BELOKUROV V. , KOPOSOV S.E.
	Mon. Not. R. Astron. Soc., 456, 602-616 (2016)
	Stellar streams around the Magellanic Clouds.
o	Figs 6-7: <[BK2016] SN> (Nos S1-S4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BK2017]
[BK2017]	(Brorby+Kaaret, 2017)
Write:	<<[BK2017] SHOC 486 X-1>> <<[BK2017] J0842 X-N>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-S observations of N=2 luminous compact galaxies SHOC 486 and SDSS J084220.94+115000.2.
in source:	SHOC 486
in source:	SDSS J084220.94+115000.3
Ref:	=2017MNRAS.470..606B
by	BRORBY M. , KAARET P.
	Mon. Not. R. Astron. Soc., 470, 606-611 (2017)
	X-rays from Green Pea analogues.
o	Table 1: <[BK2017] SHOC 486 X-1> N=1, <[BK2017] J0842 X-N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BK80]
[BK80]	(Borngen+Kalloglyan, 1980)
Write:	<<[BK80] NN>>
N:	70
Object:	G (SIMBAD class: Galaxy)
Note:	Finding charts.
Ref:	=1980Afz....16...25B
by	BORNGEN F. , KALLOGLYAN A.T.
	Astrofizika, 16, 25-28 (1980)
	Compact galaxies in a field around 07h59m +54°44'.
o	Table 1: <[BK80] NN> (Nos 1-70).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BK85
BK85	(Borngen+Karchentseva, 1985)= (BK)
Write:	<<BK85 NN>>
N:	24
Object:	Dwarf G (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	in IC 342 group. Identif. charts. See also BK in M81/82 group.
in source:	NAME IC 342 GROUP
Ref:	=1985AN....306..301B
by	BORNGEN F. , KARACHENTSEVA V.E.
	Astron. Nachr., 306, 301-304 (1985)
	Search for dwarf galaxies in the IC 342 complex of galaxies.
o	Table 2: <BK85 NN> (Nos 1-24)
Origin	of the Acronym: L (1997A&A...322..375H)
Details on Acronym: [BKB2002]
[BKB2002]	(Berger+Kulkarni+Bloom+, 2002) (Not yet in Simbad)
Write:	<<[BKB2002] GN>> <<[BKB2002] PSF Star>>
N:	3+1
Object:	G + * (SIMBAD class: Galaxy)
Note:	Image of GRB 020124 field.
Ref:	=2002ApJ...581..981B
by	BERGER E. , KULKARNI S.R., BLOOM J.S., PRICE P.A., FOX D.W., FRAIL D.A., AXELROD T.S., CHEVALIER R.A., COLBERT E., COSTA E., DJORGOVSKI S.G., FRONTERA F., GALAMA T.J., HALPERN J.P., HARRISON F.A., HOLTZMAN J., HURLEY K., KIMBLE R.A., McCARTHY P.J., PIRO L., REICHART D., RICKER G.R., SARI R., SCHMIDT B.P., WHEELER J.C., VANDERSPEK R., YOST S.A.
	Astrophys. J., 581, 981-987 (2002)
	The faint optical afterglow and host galaxy of GRB 020124: implications for the nature of dark γ-ray bursts.
o	Fig.2: Source S1 = OT 20020124.
o	Fig.1: <[BKB2002] GN> (Nos G1-G3), <[BKB2002 PSF Star> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKB2004]
[BKB2004]	(Bradley+Kaiser+Baan, 2004)= ([BKB2004a])
Write:	<<[BKB2004] Na>> <<[BKB2004] RNN>>
N:	16+10
Object:	Cloud (SIMBAD class: Cloud)
Note:	HST STIS and VLA observations of the nucleus of M 51. 9 NLR (Narrow-Line Region) Clouds with components are found, and 11 radio clouds correlated with the optical clouds.
in source:	M 51 = NGC 5194
Ref:	=2004ApJ...603..463B
by	BRADLEY L.D. , KAISER M.E., BAAN W.A.
	Astrophys. J., 603, 463-488 (2004)
	Physical conditions in the narrow-line region of M51.
o	Figs 1-3, Table 2: <[BKB2004] Na> (Nos 1-9) N=16. Figs 14-15, Table 5: <[BKB2004] ANN> (Nos R0-R10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKB2004a]
[BKB2004a]	(Bradley+Kaiser+Baan, 2004)
*****	Avoid the usage of [BKB2004a], prefer [BKB2004]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKB2004b]
[BKB2004b]	(Bratsolis+Kontizas+Bellas-Velidis, 2004)
Write:	<<[BKB2004b] NNN>>
N:	610
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Search for OB* in a region of SMC (LHA 115-N 83, 84, 85).
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2004A&A...423..919B
by	BRATSOLIS E. , KONTIZAS M., BELLAS-VELIDIS I.
	Astron. Astrophys., 423, 919-924 (2004)
	Triggered star formation in the inner wing of the SMC. Two possible supernova explosions in the N83-84-85 region.
o	Table 2 : L61-NNN = LIN NNN.
o	Table 3: <[BKB2004b] NNN> (Nos 1-610).
=E=	Catalogue in electronic form as J/A+A/423/919
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKB2006]
[BKB2006]	(Bradley+Knapen+Beckman+, 2006)= ([BKB2006a])
Write:	<<[BKB2006] NGC NNNN NNNN>>
N:	17797
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	HII region catalogues for 57 face on spiral galaxies.
Ref:	=2006A&A...459L..13B
by	BRADLEY T.R. , KNAPEN J.H., BECKMAN J.E., FOLKES S.L.
	Astron. Astrophys., 459L, 13-16 (2006)
	A composite HII region luminosity function in Hα of unprecedented statistical weight.
o	Tables hii: <[BKB2006] NGC NNNN NNNN> N=17797.
=E=	Catalogue in electronic form as J/A+A/459/L13
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKB2006a]
[BKB2006a]	(Bradley+Knapen+Beckman+, 2006)
Note:	HII region catalogues for 57 face on spiral galaxies.
*****	Avoid the usage of [BKB2006a], prefer [BKB2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKB2006b]
[BKB2006b]	(Buchkova+Kardashev+Boldycheva+, 2006)
Write:	<<[BKB2006b] GN>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	SAO 6m telescope SCORPIO observations of N=3 galaxies near S5 0716+714.
Ref:	=2006ARep...50..802B
by	BUCHKOVA V.S. , KARDASHEV N.S., BOLDYCHEVA A.V., GNEDIN Yu.N., MASLENNIKOV K.L.
	ARep, 50, 802-808 (2006)
	The unique BL Lac object S5 0716+714.
o	Fig.2: <[BKB2006b] GN> (Nos G1-G3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKB2018]
[BKB2018]	(Bhandari+Keane+Barr+, 2018)
Write:	<<[BKB2018] VLA JHHMM+DDMM>> <<[BKB2018] ATCA J2238-3011>>
N:	2+1
Object:	Variable Radio Source (SIMBAD class: Radio = Radio Source)
Note:	VLA observations of N=2 variable sources in the field of FRB 151206. ATCA observations of N=1 variable source in the field of FRB 160102.
Ref:	=2018MNRAS.475.1427B
by	BHANDARI S. , KEANE E.F., BARR E.D., JAMESON A., PETROFF E., JOHNSTON S., BAILES M., BHAT N.D.R., BURGAY M., BURKE-SPOLAOR S., CALEB M., EATOUGH R.P., FLYNN C., GREEN J.A., JANKOWSKI F., KRAMER M., VENKATRAMAN KRISHNAN V., MORELLO V., POSSENTI A., STAPPERS B., TIBURZI C., VAN STRATEN W., ANDREONI I., BUTTERLEY T., CHANDRA P., COOKE J., CORONGIU A., COWARD D.M., DHILLON V.S., DODSON R., HARDY L.K., HOWELL E.J., JAROENJITTICHAI P., KLOTZ A., LITTLEFAIR S.P., MARSH T.R., MICKALIGER M., MUXLOW T., PERRODIN D., PRITCHARD T., SAWANGWIT U., TERAI T., TOMINAGA N., TORNE P., TOTANI T., TROIS A., TURPIN D., NIINO Y., WILSON R.W., ALBERT A., ANDRE M., ANGHINOLFI M., ANTON G., ARDID M., AUBERT J.-J., AVGITAS T., BARET B., BARRIOS-MARTI J., BASA S., BELHORMA B., BERTIN V., BIAGI S., BORMUTH R., BOURRET S., BOUWHUIS M.C., BRANZAS H., BRUIJN R., BRUNNER J., BUSTO J., CAPONE A., CARAMETE L., CARR J., CELLI S., CHERKAOUI EL MOURSLI R., CHIARUSI T., CIRCELLA M., COELHO J.A.B., COLEIRO A., CONIGLIONE R., COSTANTINI H., COYLE P., CREUSOT A., DIAZ A.F., DESCHAMPS A., DE BONIS G., DISTEFANO C., DI PALMA I., DOMI A., DONZAUD C., DORNIC D., DROUHIN D., EBERL T., EL BOJADDAINI I., EL KHAYATI N., ELSASSER D., ENZENHOFER A., ETTAHIRI A., FASSI F., FELIS I., FUSCO L.A., GAY P., GIORDANO V., GLOTIN H., GREGOIRE T., GRACIA-RUIZ R., GRAF K., HALLMANN S., VAN HAREN H., HEIJBOER A.J., HELLO Y., HERNANDEZ-REY J.J., HOSSL J., HOFESTADT J., HUGON C., ILLUMINATI G., JAMES C.W., DE JONG M., JONGEN M., KADLER M., KALEKIN O., KATZ U., KIESSLING D., KOUCHNER A., KRETER M., KREYKENBOHM I., KULIKOVSKIY V., LACHAUD C., LAHMANN R., LEFEVRE D., LEONORA E., LOUCATOS S., MARCELIN M., MARGIOTTA A., MARINELLI A., MARTINEZ-MORA J.A., MELE R., MELIS K., MICHAEL T., MIGLIOZZI P., MOUSSA A., NAVAS S., NEZRI E., ORGANOKOV M., PAVALAS G.E., PELLEGRINO C., PERRINA C., PIATTELLI P., POPA V., PRADIER T., QUINN L., RACCA C., RICCOBENE G., SANCHEZ-LOSA A., SALDANA M., SALVADORI I., SAMTLEBEN D.F.E., SANGUINETI M., SAPIENZA P., SCHUSSLER F., SIEGER C., SPURIO M., STOLARCZYK T., TAIUTI M., TAYALATI Y., TROVATO A., TURPIN D., TONNIS C., VALLAGE B., VAN ELEWYCK V., VERSARI F., VIVOLO D., VIZZOCCA A., WILMS J., ZORNOZA J.D., ZUNIGA J.
	Mon. Not. R. Astron. Soc., 475, 1427-1446 (2018)
	The SUrvey for Pulsars and Extragalactic Radio Bursts - II. New FRB discoveries and their follow-up.
o	Table 3: <[BKB2018] VLA JHHMM+DDMM> N=2, <[BKB2018] ATCA J2238-3011> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKB95]
[BKB95]	(Beers+Kriessler+Bird+, 1995)
Write:	<<[BKB95] HHMM+DDMMA>>
N:	812
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	G in 23 poor clusters.
Ref:	=1995AJ....109..874B
by	BEERS T.C. , KRIESSLER J.R., BIRD C.M., HUCHRA J.P.
	Astron. J., 109, 874-919 (1995)
	Kinematics and dynamics of the MKW/AWM poor clusters.
o	Table 2: <[BKB95] HHMM+DDMMA> N=812
=E=	Catalogue in electronic form as J/AJ/109/874
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKB99]
[BKB99]	(Becker+Kawai+Brinkmann+, 1999)
Write:	<<[BKB99] PSR B1055-52 CN>> <<[BKB99] PSR B1055-52 NN>> <<[BKB99] PSR B0656+14 CN>> <<[BKB99] PSR B0656+14 NN>> <<[BKB99] Geminga CN>> <<[BKB99] Geminga NN>>
N:	3+13+2+15+8+23
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Analysis of archival ASCA, ROSAT and BeppoSAX data around PSR B1055-52, PSR B0656+14, and Geminga pulsar. PSR B1055-52: (Nos C1-C2, C4), X-ray sources observed from BeppoSAX. Map Fig.2. Sources C1 and C2 were interpreted as clumps in [SSG97], from ASCA observations. (Nos 1-13), X-ray sources observed from ROSAT PSPC. Map Fig.3. PSR B0656+14: (Nos C1-C3), X-ray sources observed from ASCA. Map Fig.5. (Nos 1-15), X-ray sources observed from ROSAT PSPC. Map Fig.6. Geminga: (Nos C1-C8), X-ray sources observed from ASCA. Map Fig.8. (Nos 1-23), X-ray sources observed from ROSAT PSPC. Map Fig.9.
Ref:	=1999A&A...352..532B
by	BECKER W. , KAWAI N., BRINKMANN W., MIGNANI R.
	Astron. Astrophys., 352, 532-542 (1999)
	The putative pulsar-wind nebulae of the three Musketeers PSR B1055-52, B0656+14 and Geminga revisited.
o	Table 1: <[BKB99] PSR B1055-52 CN> (Nos C1-C2, C4). Table 2: <[BKB99] PSR B1055-52 NN> (Nos 1-13). Table 3: <[BKB99] PSR B0656+14 CN> (Nos C1-C3), <[BKB99] PSR B0656+14 NN> (Nos 1-15). Table 4: <[BKB99] Geminga CN> (Nos C1-C8), <[BKB99] Geminga NN> (Nos 1-23).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKC98]
[BKC98]	(Brouillet+Kaufman+Combes+, 1998)
Write:	<<[BKC98] CN>>
N:	6
Object:	Molecular Complex (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=6 molecular Complexes (letter 'C' in the format) in M 81 Identif chart in Fig.6
in source:	M 81 = NGC 3031
Ref:	=1998A&A...333...92B
by	BROUILLET N. , KAUFMAN M., COMBES F., BAUDRY A., BASH F.
	Astron. Astrophys., 333, 92-100 (1998)
	Identification of molecular complexes in M 81.
o	HII regions 138 and 172 in M81 are [KBK87] 138, 172 in SIMBAD
o	Table 1: <[BKC98] CN> (Nos C1-C6)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKD2005]
[BKD2005]	(Buckalew+Kobulnicky+Dufour, 2005)
Write:	<<[BKD2005] R Zw NN>> <<[BKD2005] Mrk NNN>> <<[BKD2005] Mrk NNNN N>> <<[BKD2005] NGC NNNN NN>> <<[BKD2005] UM NNN N>>
N:	42
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	KPNO and San Pedro Martir observations, with complementary observations from HST and 2MASS. Search for stellar clusters in 14 galaxies.
Ref:	=2005ApJS..157...30B
by	BUCKALEW B.A. , KOBULNICKY H.A., DUFOUR R.J.
	Astrophys. J., Suppl. Ser., 157, 30-58 (2005)
	Comparison of star clusters with and without Wolf-Rayet stars in Wolf-Rayet galaxies.
o	Table 15: Tol 1004-286 is a misprint for Tol 1004-296
o	Table 3: <[BKD2005] I Zw 18>, <[BKD2005] II Zw 40>, <[BKD2005] Mrk 475>, <[BKD2005] Mrk NNNN N>, <[BKD2005] NGC NNNN NN>, <[BKD2005] UM 311 N>, N=42.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKD2006]
[BKD2006]	(Buckalew+Kobulnicky+Darnel+, 2006) (Not yet in Simbad)
Write:	<<[BKD2006] NNa>>
N:	23
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	UV, Optical, NIR, Spitzer mid-IR and radio images of 14 radio selected objects in M 33.
in source:	M 33 = NGC 598
Ref:	=2006ApJS..162..329B
by	BUCKALEW B.A. , KOBULNICKY H.A., DARNEL J.M., POLOMSKI E., GEHRZ R.D., HUMPHREYS R.M., WOODWARD C.E., HINZ J.L., ENGELBRACHT C.W., GORDON K.D., MISSELT K., PEREZ-GONZALEZ P.G., RIEKE G.H., WILLNER S.P., ASHBY M.L., BARMBY P., PAHRE M.A., ROELLIG T.L., DEVEREUX N., LOON J.T., BRANDL B.
	Astrophys. J., Suppl. Ser., 162, 329-345 (2006)
	Understanding radio-selected thermal sources in M 33: ultraviolet, optical, near-infrared, Spitzer mid-infrared, and radio observations.
o	Table 2: <[BKD2006] NNa> N=23, (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKD2008]
[BKD2008]	(Brinchmann+Kunth+Durret, 2008)
Write:	<<[BKD2008] WR NNN>>
N:	570
Object:	G + Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Analysis of the properties of galaxies showing Wolf-Rayet features in their optical spectrum using specra from the SDDSS DR6.
Ref:	=2008A&A...485..657B
by	BRINCHMANN J. , KUNTH D., DURRET F.
	Astron. Astrophys., 485, 657-677 (2008)
	Galaxies with Wolf-Rayet signatures in the low-redshift Universe. A survey using the Sloan Digital Sky Survey.
o	Table 3: <[BKD2008] WR NNN> (Nos 0-569).
=E=	Catalogue in electronic form as J/A+A/485/657
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKD2020]
[BKD2020]	(Bait+Kurapati+Duc+, 2020)
Write:	<<[BKD2020] HI Ring>> <<[BKD2020] OCN>>
N:	1+5
Object:	HI + (Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	GMRT 21-cm and CFHT MegaCam optical observations of N=1 HI ring and N=5 optical counterpart candidates in the field of AGC 203001.
Ref:	=2020MNRAS.492....1B
by	BAIT O. , KURAPATI S., DUC P.-A., CUILLANDRE J.-C., WADADEKAR Y., KAMPHUIS P., BARWAY S.
	Mon. Not. R. Astron. Soc., 492, 1-7 (2020)
	Discovery of a large H I ring around the quiescent galaxy AGC 203001.
o	Figs 1- 2, Table 2: <[BKD2020] HI Ring> N=1, <[BKD2020] OCN> (Nos OC1-OC5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKF2005]
[BKF2005]	(Berger+Kulkarni+Fox+, 2005)
Write:	<<[BKF2005] GRB YYMMDD abs N.NNNN>>
N:	1+2+1
Object:	Absorber
Note:	Magellan 6.5m telescopes LDSS3 and IMACS absorption spectrum of GRB 050315, GRB 050318, GRB 050408.
Ref:	=2005ApJ...634..501B
by	BERGER E. , KULKARNI S.R., FOX D.B., SODERBERG A.M., HARRISON F.A., NAKAR E., KELSON D.D., GLADDERS M.D., MULCHAEY J.S., OEMLER A., DRESSLER A., CENKO S.B., PRICE P.A., SCHMIDT B.P., FRAIL D.A., MORRELL N., GONZALEZ S., KRZEMINSKI W., SARI R., GAL-YAM A., MOON D.-S., PENPRASE B.E., JAYAWARDHANA R., SCHOLZ A., RICH J., PETERSON B.A., ANDERSON G., McNAUGHT R., MINEZAKI T., YOSHII Y., COWIE L.L., PIMBBLET K.
	Astrophys. J., 634, 501-508 (2005)
	Afterglows, redshifts, and properties of Swift γ-ray bursts.
o	Fig.1: <[BKF2005] GRB 050315 abs N.NNNN> N=1. Fig.2: <[BKF2005] GRB 050318 abs N.NNNN> N=2. Fig.3: <[BKF2005] GRB 050408 abs N.NNNN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKF98]
[BKF98]	(Bresolin+Kennicutt+Ferrarese+, 1998)
Write:	<<[BKF98] NGC NNNN NN>>
N:	21+17+6+9
Object:	Poss. * Cluster (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST observations of 4 galaxies, searching for OB associations.
in source:	NGC 3621
in source:	NGC 925
in source:	NGC 2541
in source:	NGC 3351
Ref:	=1998AJ....116..119B
by	BRESOLIN F. , KENNICUTT R.C.Jr, FERRARESE L., GIBSON B.K., GRAHAM J.A., MACRI L.M., PHELPS R.L., RAWSON D.M., SAKAI S., SILBERMANN N.A., STETSON P.B., TURNER A.M.
	Astron. J., 116, 119-130 (1998)
	A Hubble Space Telescope study of extragalactic OB Associations.
o	Table 3: <[BKF98] NGC 3621 NN> (Nos 1-21), <[BKF98] NGC 925 NN> (Nos 1-17), <[BKF98] NGC 2541 N> (Nos 1-6), <[BKF98] NGC 3351 N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKG2004]
[BKG2004]	(Borissova+Kurtev+Georgiev+, 2004)
Write:	<<[BKG2004] GNN>>
N:	60
Object:	OB Assoc. (SIMBAD class: Association = Association of Stars)
Stat:	is completely incorporated in Simbad
Note:	Bulgarian National Astronomical Observatory and San Pedro Martir observations. Catalogue of OB association in IC 1613.
in source:	IC 1613
Ref:	=2004A&A...413..889B
by	BORISSOVA J. , KURTEV R., GEORGIEV L., ROSADO M.
	Astron. Astrophys., 413, 889-893 (2004)
	A catalogue of OB associations in IC 1613.
o	Table 1 : Hodge Associations are [H78] Ass NN in Simbad.
o	Table 1: <[BKG2004] GNN> (Nos G1-G60).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKG2010]
[BKG2010]	(Berciano Alba+Koopmans+Garrett+, 2010)
Write:	<<[BKG2010] RJ>> <<[BKG2010] CRN>> <<[BKG2010] EN>> <<[BKG2010] NN>>
N:	6+27
Object:	(Rad) + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	VLA 1.4GHz observations of the cluster MS0451.6-0305.
in source:	ClG 0451-0305 = 1E 0451.6-0305
Ref:	=2010A&A...509A..54B
by	BERCIANO ALBA A. , KOOPMANS L.V.E., GARRETT M.A., WUCKNITZ O., LIMOUSIN M.
	Astron. Astrophys., 509A, 54-54 (2010)
	Radio counterpart of the lensed submm emission in the cluster MS0451.6-0305: new evidence for the merger scenario.
o	Fig. 4, Table 1: <[BKG2010] AAN> (Nos RJ, CR1-CR2, E1-E3). Fig. 5, Table 12: <[BKG2010] NN> (Nos 1-27).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKG2013]
[BKG2013]	(Buchbender+Kramer+Gonzalez-Garcia+, 2013)
Write:	<<[BKG2013] M33noN>>
N:	4 (SIMBAD class: MolCld = Molecular Cloud)
Note:	IRAM 30m CO, HCO+, HCN, and HNC observations of M 33.
in source:	M 33
Ref:	=2013A&A...549A..17B
by	BUCHBENDER C. , KRAMER C., GONZALEZ-GARCIA M., ISRAEL F.P., GARCIA-BURILLO S., VAN DER WERF P., BRAINE J., ROSOLOWSKY E., MOOKERJEA B., AALTO S., BOQUIEN M., GRATIER P., HENKEL C., QUINTANA-LACACI G., VERLEY S., VAN DER TAK F.
	Astron. Astrophys., 549A, 17-17 (2013)
	Dense gas in M 33 (HerM33es).
o	Table 2 : <[BKG2013] M33noN> N=4 among (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKG99]
[BKG99]	(Bresolin+Kennicutt+Garnett, 1999)
Write:	<<[BKG99] M NN NN>> <<[BKG99] NGC NNNN N>>
N:	96
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	N=96 giant HII regions distributed in 20 spiral galaxies.
Ref:	=1999ApJ...510..104B
by	BRESOLIN F. , KENNICUTT R.C.Jr, GARNETT D.R.
	Astrophys. J., 510, 104-124 (1999)
	The ionizing stars of extragalactic H II regions.
o	cross-id. HK = HK NGC, H = [H76], P = [PAV78], CCM, GS = [GS87], D = [DTJ80], Munch = [M59b].
o	Table 3: <[BKG99] M NN NN>, <[BKG99] NGC NNNN N>, N=96.
=E=	Catalogue in electronic form as J/ApJ/510/104
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BKGS
BKGS	(Bruhweiler+Klinglesmith+Gull+Sofia)
Write:	<<BKGS NNA>>
N:	37
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-35) Several identif. on Fig. 1 are lacking or erroneous for sources 20 to 35. A few sources have not been detected later by Wang+Wu (ref. 1992ApJS...78..391W, Table 2C) Fig. 1: Identif. chart
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1987ApJ...317..152B
by	BRUHWEILER F.C. , KLINGLESMITH III D.A., GULL T.R., SOFIA S.
	Astrophys. J., 317, 152-162 (1987)
	Deep Einstein X-ray imagery of the Small Magellanic Cloud.
o	Table 2: <BKGS NNA> (Nos 1A-1B, 2-17, 18A-18B, 19-35)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BKH2005]
[BKH2005]	(Bik+Kaper+Hanson+, 2005)= ([BKH2005a])
Write:	<<[BKH2005] HHMMmnrNNNNA>>
N:	50+29+1
Object:	* (SIMBAD class: Star)
Note:	ISAAC ESO-VLT spectral observations of point sources in IRAS UCHII regions. HHMMm in the format stands for the IRAS HHMMm+DDMM region.
Ref:	=2005A&A...440..121B
by	BIK A. , KAPER L., HANSON M.M., SMITS M.
	Astron. Astrophys., 440, 121-137 (2005)
	VLT K-band spectroscopy of massive stars deeply embedded in IRAS sources with UCHII colours.
o	Table 4 17175nr57 is a probable misprint for [BKH2005] 17175nr59
o	Tables 3, 4, 5: <[BKH2005] HHMMmnrNNNNA> N=50.
Ref:	=2006A&A...455..561B
by	BIK A. , KAPER L., WATERS L.B.F.M.
	Astron. Astrophys., 455, 561-576 (2006)
	VLT K-band spectroscopy of massive young stellar objects in (ultra-)compact HII regions.
o	Table 3, text: <[BKH2005] HHMMmnrNNNNA> N=29 added.
Ref:	=2013A&A...551A...5E
by	ELLERBROEK L.E. , PODIO L., KAPER L., SANA H., HUPPENKOTHEN D., DE KOTER A., MONACO L.
	Astron. Astrophys., 551A, 5-5 (2013)
	The outflow history of two Herbig-Haro jets in RCW 36: HH 1042 and HH 1043.
o	<[BKH2005] HHMMmnrNNNN> (No. 08576nr480) added.
=E=	Catalogue in electronic form as <J/A+A/440/121/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKH2005a]
[BKH2005a]	(Bik+Kaper+Hanson+, 2005)
*****	Avoid the usage of [BKH2005a], prefer [BKH2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKH2005b]
[BKH2005b]	(BEST+Kauffman+Heckman+, 2005)
Write:	<<[BKH2005b] DDD.ddddd+D.dddd>>
N:	2709
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	2712 radio-luminous galaxies from the DR2 SDSS, compared with NVSS and FIRST surveys.
Ref:	=2005MNRAS.362....9B
by	BEST P.N. , KAUFFMANN G., HECKMAN T.M., IVEZIC Z.
	Mon. Not. R. Astron. Soc., 362, 9-24 (2005)
	A sample of radio-loud active galactic nuclei in the Sloan Digital Sky Survey.
o	Table 2: <[BKH2005b] DDD.ddddd+D.dddd> N=2709.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKH2007]
[BKH2007]	(Birkmann+Krause+Hennemann+, 2007)
Write:	<<[BKH2007] ISOSS J23053+5953 SMMNa>>
N:	2+3
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SCUBA observations of ISOPHOT Serendipity Survey (ISOSS) sources.
in source:	ISOSS J23053+5953
Ref:	=2007A&A...474..883B
by	BIRKMANN S.M. , KRAUSE O., HENNEMANN M., HENNING T., STEINACKER J., LEMKE D.
	Astron. Astrophys., 474, 883-890 (2007)
	A massive protostellar core with an infalling envelope.
o	Fig.3, Table 2: <[BKH2007] ISOSS J23053+5953 SMMNa> (Nos 1-2, 1a-1c).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKH2010]
[BKH2010]	(BEERER+KOENIG+HORA+, 2010)
Write:	<<[BKH2010] GLL.ll+B.bb>> <<[BKH2010] JHHMMSS.ss+DDMMSS.s>>
N:	13+6+536
Object:	Cluster of * + YSO (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC and MIPS observations of Cygnus X North.
Ref:	=2010ApJ...720..679B
by	BEERER I.M. , KOENIG X.P., HORA J.L., GUTERMUTH R.A., BONTEMPS S., MEGEATH S.T., SCHNEIDER N., MOTTE F., CAREY S., SIMON R., KETO E., SMITH H.A., ALLEN L.E., FAZIO G.G., KRAEMER K.E., PRICE S., MIZUNO D., ADAMS J.D., HERNANDEZ J., LUCAS P.W.
	Astrophys. J., 720, 679-693 (2010)
	A Spitzer view of star formation in the Cygnus X North complex.
o	Tables 4,6: <[BKH2010] GLL.ll+B.bb> N=13+6, Table 7: <[BKH2010] JHHMMSS.ss+DDMMSS.s> N=536
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKH2014]
[BKH2014]	(Babusiaux+Katz+Hill+, 2014)
Write:	<<[BKH2014] 9P NNNNN>> <<[BKH2014] 5PN NNNNN>> <<[BKH2014] C32 NNNNN>> <<[BKH2014] 5NN NNNNN>>
N:	92+101+107+99
Object:	* (SIMBAD class: Star)
Note:	VLT FLAMES GIRAFFE low-resolution spectroscopy of N=92+101+107+99 red clump giant candidates in four fields located along the Galactic bar major axis.
in source:	NAME Galactic Bulge
Ref:	=2014A&A...563A..15B
by	BABUSIAUX C. , KATZ D., HILL V., ROYER F., GOMEZ A., ARENOU F., COMBES F., DI MATTEO P., GILMORE G., HAYWOOD M., ROBIN A.C., RODRIGUEZ-FERNANDEZ N., SARTORETTI P., SCHULTHEIS M.
	Astron. Astrophys., 563A, 15-15 (2014)
	Metallicity and kinematics of the bar in situ.
o	Table 2: <[BKH2014] 9P NNNNN> N=92 among (Nos 00002-00182), <[BKH2014] 5PN NNNNN> N=101 among (Nos 00003-00193), <[BKH2014] C32 NNNNN> N=107 among (Nos 00004-00326), <[BKH2014] 5NN NNNNN> N=99 among (Nos 00001-00271).
=E=	Catalogue in electronic form as J/A+A/563/A15
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BKK
BKK	(Borngen+Karachentseva+Karachentsev)
Write:	<<BKK NN>>
N:	11
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
in source:	NAME M 81 GROUP
Ref:	=1984AN....305...53B
by	BORNGEN F. , KARACHENTSEVA V.E., KARACHENTSEV I.D.
	Astron. Nachr., 305, 53-57 (1984)
	An unusual group of low surface brightness galaxies in the region 1046+65.
o	Table I: <BKK NN> (Nos 1-11)
Origin	of the Acronym: L (1998A&AS..129..313B)
Details on Acronym: [BKL2006]
[BKL2006]	(Birkmann+Krause+Lemke, 2006)= (SMM)
Write:	<<[BKL2006] ISOSS J18364-0221 SMM N>>
N:	2
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	Discovery of two cold and massive molecular clouds cores in the region of ISOSS J18364-0221, using the 170mu.m ISOPHOT Serendipity Survey (ISOSS)
Ref:	=2006ApJ...637..380B
by	BIRKMANN S.M. , KRAUSE O., LEMKE D.
	Astrophys. J., 637, 380-383 (2006)
	Very cold and massive cores near ISOSS J18364-0221: implications for the initial conditions of high-mass star formation.
o	Figs: <[BKL2006] ISOSS J18364-0221 SMM N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BKLT
BKLT	(Barsony+Kenyon+Lada+Teuben)= (B)
Write:	<<BKLT JHHMMSS+DDMMSSA>>
N:	4495
Object:	(Near IR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Stat:	is completely incorporated in Simbad
Note:	The BKLT catalog lists positions (both J2000.0 and B1950.0) to 1.2" accuracy and JHK magnitudes for 4495 sources identified from a near-infrared imaging survey (using the SQIID instrument on the KPNO 1.3-meter telescope) which covered a square degree of the star-forming rho Ophiuchi cloud core.
in source:	NAME rho Oph Cloud
Ref:	=1997ApJS..112..109B
by	BARSONY M. , KENYON S.J., LADA E.A., TEUBEN P.J.
	Astrophys. J., Suppl. Ser., 112, 109-191 (1997)
	A near-infrared imaging survey of the ρ Ophiuchi cloud core.
o	Table 2: <BKLT JHHMMSS-DDMMSSA> N=4495.
=E=	Catalogue in electronic form as J/ApJS/112/109
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BKM2001]
[BKM2001]	(Bresolin+Kudritzki+Mendez+, 2001)
Write:	<<[BKM2001] NN>> <<[BKM2001] Star a>>
N:	19
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	FORS ESO VLT observations. Spectroscopy of NGC 3621. N=19 objects, among which HII regions and 3 stars (Nos a-c).
in source:	NGC 3621
Ref:	=2001ApJ...548L.159B
by	BRESOLIN F. , KUDRITZKI R.-P., MENDEZ R.H., PRZYBILLA N.
	Astrophys. J., 548, 159-163 (2001)
	Stellar spectroscopy far beyond the Local Group.
o	Fig.1, Table 1: <[BKM2001] NN> (Nos 1-19), <[BKM2001] Star a> (Nos a-c).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKM2005]
[BKM2005]	(Boles+Khandrika+Madison+, 2005)
Write:	<<[BKM2005] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of SN 2005EJ.
Ref:	=2005IAUC.8604....1B
by	BOLES T. , (LOSS/KAIT), KHANDRIKA H., MADISON D.R., BAEK M., SHIMASAKI K., LI W.
	IAU Circ., 8604, 1-None (2005)
	Supernovae 2005ej, 2005ek, 2005el, 2005em.
o	<[BKM2005] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKM2008]
[BKM2008]	(Bouvier+Kendall+Meeus+, 2008)
Write:	<<[BKM2008] HANNcNN-NNNNa>> <<[BKM2008] HANIcNN-NNNNa>>
N:	22+103
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	CFHT photometric survey of the Hyades cluster region. Probable non-members.
in source:	Hyades = Cl Melotte 25
Ref:	=2008A&A...481..661B
by	BOUVIER J. , KENDALL T., MEEUS G., TESTI L., MORAUX E., STAUFFER J.R., JAMES D., CUILLANDRE J.-C., IRWIN J., McCAUGHREAN M.J., BARAFFE I., BERTIN E.
	Astron. Astrophys., 481, 661-672 (2008)
	Brown dwarfs and very low mass stars in the Hyades cluster: a dynamically evolved mass function.
o	Paragraph 3.2 LH 0420+15 is an incomplete format. Can be [LHD94] 042011.2+150645, [LHD94] 042021.6+153550, [LHD94] 042033.9+153453 or [LHD94] 042051.9+154557.
o	Table 1, col(1): <Cl* Melotte 25 CFHT NN> (Nos 1-21). Table 1, col(2), Table D1: <[BKM2008] HANNcNN-NNNNa>, <[BKM2008] HANIcNN-NNNNa> N=22+103.
=E=	Catalogue in electronic form as J/A+A/481/661
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKM2016]
[BKM2016]	(Belardi+Kilic+Munn+, 2016)
Write:	<<[BKM2016] WDNNN>>
N:	111
Object:	Poss. WD (SIMBAD class: WhiteDwarf_Candidate = White Dwarf Candidate)
Note:	CTIO Blanco telescope DECam observations of N=111 high proper motion white dwarf candidates.
Ref:	=2016MNRAS.462.2506B
by	BELARDI C. , KILIC M., MUNN J.A., GIANNINAS A., BARBER S.D., DEY A., STETSON P.B.
	Mon. Not. R. Astron. Soc., 462, 2506-2517 (2016)
	The DECam Minute Cadence Survey - I.
o	Tables 1-4: <[BKM2016] WDNNN> N=111 among (Nos 1-112), No. 104 missing.
=E=	Catalogue in electronic form as <J/MNRAS/462/2506/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKM2020]
[BKM2020]	(Bosman+Kakiichi+Meyer+, 2020)
Write:	<<[BKM2020] Aerith A>>
N:	3
Object:	LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Subaru SuprimeCam photometry and Keck II DEIMOS spectroscopy of N=3 Lyman α emitters (LAEs) in the proximity zone of quasar SDSS J083643.85+005453.3.
Ref:	=2020ApJ...896...49B
by	BOSMAN S.E.I. , KAKIICHI K., MEYER R.A., GRONKE M., LAPORTE N., ELLIS R.S.
	Astrophys. J., 896, 49-49 (2020)
	Three Lyα emitting galaxies within a quasar proximity zone at z ~ 5.8.
o	Fig. 1, Table 2: <[BKM2020] Aerith A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKM2021]
[BKM2021]	(Bhardwaj+Kirichenko+Michilli+, 2022)
Write:	<<[BKM2021] N>>
N:	7
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	GTC OSIRIS observations of N=7 galaxies in the field of FRB 20181030A. Use of DESI Legacy Imaging Survey data.
Ref:	=2021ApJ...919L..24B
by	BHARDWAJ M. , KIRICHENKO A.Y., MICHILLI D., MAYYA Y.D., KASPI V.M., GAENSLER B.M., RAHMAN M., TENDULKAR S.P., FONSECA E., JOSEPHY A., LEUNG C., MERRYFIELD M., PETROFF E., PLEUNIS Z., SANGHAVI P., SCHOLZ P., SHIN K., SMITH K.M., STAIRS I.H.
	Astrophys. J., 919L, 24-24 (2021)
	A local universe host for the repeating fast radio burst FRB 20181030A.
o	Fig. 2, Table 4: <[BKM2021] N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKN2000]
[BKN2000]	(Baba+Kato+Nogami+, 2000)
Write:	<<[BKN2000] CN>> <<[BKN2000] aN>>
N:	3+3
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=3 comparison stars (Nos C1-C3) and N=3 check stars (Nos a1-a3) in the field of V1028 Cyg. Finding chart in Fig.1.
Ref:	=2000PASJ...52..429B
by	BABA H. , KATO T., NOGAMI D., HIRATA R., MATSUMOTO K.
	Publ. Astron. Soc. Jap., 52, 429-436 (2000)
	Discovery of a new SU UMa-type dwarf nova, V1028 Cygni.
o	Table 2: <[BKN2000] CN> (Nos C1-C3), <[BKN2000] aN> (Nos a1-a3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BKP
BKP	(Brunt+Kerton+Pomerleau)
*****	Avoid the usage of BKP, prefer [BKP2003]
Origin	of the Acronym: L (2002AJ....124.3449K)
Details on Acronym: [BKP2002]
[BKP2002]	(Bloom+Kulkarni+Price+, 2002)= ([BKP2002a])
Write:	<<[BKP2002] A>>
N:	2
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST image of GRB 011121: 2 point sources are present in the field, probably foreground stars.
Ref:	=2002ApJ...572L..45B
by	BLOOM J.S. , KULKARNI S.R., PRICE P.A., REICHART D., GALAMA T.J., SCHMIDT B.P., FRAIL D.A., BERGER E., McCARTHY P.J., CHEVALIER R.A., WHEELER J.C., HALPERN J.P., FOX D.W., DJORGOVSKI S.G., HARRISON F.A., SARI R., AXELROD T.S., KIMBLE R.A., HOLTZMAN J., HURLEY K., FRONTERA F., PIRO L., COSTA E.
	Astrophys. J., 572, 45-49 (2002)
	Detection of a supernova signature associated with GRB 011121.
o	Fig.1: <[BKP2002] A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKP2002a]
[BKP2002a]	(Bloom+Kulkarni+Price+, 2002)
*****	Avoid the usage of [BKP2002a], prefer [BKP2002]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKP2002b]
[BKP2002b]	(Beuther+Kerp+Preibisch+, 2002)
Write:	<<[BKP2002b] XNN>>
N:	13
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of the star-forming region IRAS 19410+2336.
in source:	IRAS 19410+2336
Ref:	=2002A&A...395..169B
by	BEUTHER H. , KERP J., PREIBISCH T., STANKE T., SCHILKE P.
	Astron. Astrophys., 395, 169-177 (2002)
	Hard X-ray emission from a young massive star-forming cluster.
o	Table 1: <[BKP2002b] XNN> (Nos X1-X13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKP2003]
[BKP2003]	(Brunt+Kerton+Pomerleau, 2003)= (BKP)
Write:	<<[BKP2003] NNNNN>> <<[BKP2003] OIN NNNN>>
N:	14595
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	Catalog of molecular clouds generated from the Five College Radio Astronomy Observatory Galaxy Survey of 12CO (J = 1-0) emission using a two-phase object identification procedure. In the first phase, continuous emission structures are detected, designated as 'OIN' (Object Identification Number) by the authors, resulting in 9489 objects. In the second phase, a total of 14595 'Subobjects' (SIN for the authors) are detected, then simply designated as the objects of the catalog.
Ref:	=2003ApJS..144...47B
by	BRUNT C.M. , KERTON C.R., POMERLEAU C.
	Astrophys. J., Suppl. Ser., 144, 47-70 (2003)
	An outer galaxy molecular cloud catalog.
o	Objects SIN NNNNN are [BKP2003] NNNNN in SIMBAD, Objects OIN NNNN are [BKP2003] OIN NNNN.
o	Table 3: <[BKP2003] NNNNN> (Nos 4-14595). Table 3, col(2): <[BKP2003] OIN NNNN> (Nos 4-9489).
=E=	Catalogue in electronic form as J/ApJS/144/47
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKP2013]
[BKP2013]	(Benaglia+Koribalski+Peri+, 2013)
Write:	<<[BKP2013] a>> <<[BKP2013] ddN>>
N:	5+3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA 5.5GHz continuum observations of N=5+3 discrete isolated radio sources in the field surrounding RCW 49. The double source dd, composed of dd1 and dd2, was also detected at 9.0GHz.
in source:	RCW 49
Ref:	=2013A&A...559A..31B
by	BENAGLIA P. , KORIBALSKI B., PERI C.S., MARTI J., SANCHEZ-SUTIL J.R., DOUGHERTY S.M., NORIEGA-CRESPO A.
	Astron. Astrophys., 559A, 31-31 (2013)
	High-resolution radio emission from RCW 49/Westerlund 2.
o	Fig. 4, Table 2: <[BKP2013] a> (Nos a-c, e-f), <[BKP2013] ddN> (Nos dd, dd1-dd2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKR2012]
[BKR2012]	(BRESOLIN+KENNICUTT+RYAN-WEBER, 2012)
Write:	<<[BKR2012] JHHMMSS.ss+DDMMSS.s>> <<[BKR2012] NGC1512 NN>> <<[BKR2012] NGC3621 NN>>
N:	142
Object:	HII + Em* + SNR (SIMBAD class: PartofG = Part of a Galaxy)
Note:	VLT FORS2 observations of NGC 1512 and NGC 3621.
in source:	NGC 1512
in source:	NGC 3621
Ref:	=2012ApJ...750..122B
by	BRESOLIN F. , KENNICUTT R.C., RYAN-WEBER E.
	Astrophys. J., 750, 122 (2012)
	Gas metallicities in the extended disks of NGC 1512 and NGC 3621. Chemical signatures of metal mixing or enriched gas accretion?
o	Table 2: <[BKR2012] JHHMMSS.ss+DDMMSS.s> N=7, Table 5: <[BKR2012] NGC1512 NN> (Nos 1-62), Table 6: <[BKR2012] NGC3621 NN> (Nos 1-73).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKS95]
[BKS95]	(Bahcall+Kirhakos+Schneider+, 1995)
Write:	<<[BKS95] A>> <<[BKS95] AN>> <<[BKS95] {In\|Ex}N>>
N:	6+13
Object:	Knot (SIMBAD class: PartofCloud = Part of Cloud)
Note:	HST, MERLIN and CHANDRA observations Knot H is divided into (H1-H3) sub-components, [BKS95] H1, 2, 3 = [FC85] 1, 2, 3 respectively. Knots In1, In2, and Ex1 (for Internal and External).
in source:	3C 273
Ref:	=1995ApJ...452L..91B
by	BAHCALL J.N. , KIRHAKOS S., SCHNEIDER D.P., UNWIN S.C.
	Astrophys. J., 452, 91-93 (1995)
	Hubble Space Telescope and MERLIN observations of the jet in 3C 273.
o	<[BKS95] A> (Nos A-D, F, H), <[BKS95] AN> (Nos A1-A3, B1-B2, C1-C3, H1-H3), <[BKS95] InN> (Nos In1-In2), <[BKS95] Ex1>
Ref:	=2001ApJ...549L.161S
by	SAMBRUNA R.M. , URRY C.M., TAVECCHIO F., MARASCHI L., SCARPA R., CHARTAS G., MUXLOW T.
	Astrophys. J., 549, 161-165 (2001)
	Chandra observations of the X-ray jet of 3C 273.
o	<[BKS95] AN> (Nos D1-D3) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKS96]
[BKS96]	(Bresolin+Kennicutt+Stetson, 1996)= ([BKS96a])
Write:	<<[BKS96] OB NN>> <<[BKS96] Cl NN>>
N:	79+43
Object:	OB Assoc. + Cluster of * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Investigation of an HST field in M 101 Table 2: N=79 OB Assoc., format 'OB NN' Table 6: N=43 stellar clusters, format 'Cl NN'
in source:	M 101 = NGC 5457
Ref:	=1996AJ....112.1009B
by	BRESOLIN F. , KENNICUTT R.C.Jr, STETSON P.B.
	Astron. J., 112, 1009-1020 (1996)
	An HST study of OB associations and star clusters in M101.
o	Table 2: <[BKS96] OB NN> (Nos 1-79). Table 6: <[BKS96] Cl NN> (Nos 1-43)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKS96a]
[BKS96a]	(Bresolin+Kennicutt+Stetson, 1996)
*****	Avoid the usage of [BKS96a], prefer [BKS96]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKS96b]
[BKS96b]	(Bahcall+Kirhakos+Schneider+, 1996)
Write:	<<[BKS96b] PHL 909 A>> <<[BKS96b] PG 0052+251 A>> <<[BKS96b] PG 0052+251 a>>
N:	10+7+11
Object:	G + HII (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations Maps in Plate 6 for HII regions
in source:	PHL 909
in source:	PG 0052+251
Ref:	=1996ApJ...457..557B
by	BAHCALL J.N. , KIRHAKOS S., SCHNEIDER D.P.
	Astrophys. J., 457, 557-564 (1996)
	The apparently normal galaxy hosts for two luminous quasars.
o	Table 3: <[BKS96b] PHL 909 A> (Nos A-J). Table 4: <[BKS96b] PG 0052+251 A> (Nos A-G). Table 5: <[BKS96b] PG 0052+251 a> (Nos a-k)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKS97]
[BKS97]	(Beaulieu+Krochenberger+Sasselov+, 1997)= (EROS)
Write:	<<[BKS97] NNNN>>
N:	11
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	The format 'NNNN' used is an intermediary numbering used in the EROS database. See EROS final catalogue in the SMC.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1997A&A...321L...5B
by	BEAULIEU J.P. , KROCKENBERGER M., SASSELOV D.D., RENAULT C., FERLET R., VIDAL-MADJAR A., MAURICE E., PREVOT L., AUBOURG E., BAREYRE P., BREHIN S., COUTURES C., DELABROUILLE N., DE KAT J., GROS M., LAURENT B., LACHIEZE-REY M., LESQUOY E., MAGNEVILLE C., MILSZTAJN A., MOSCOSO L., QUEINNEC F., RICH J., SPIRO M., VIGROUX L., ZYLBERAJCH S., ANSARI R., CAVALIER F., MONIEZ M., GRY C.
	Astron. Astrophys., 321, 5-8 (1997)
	EROS VARIABLE STARS: Discovery of beat Cepheids in the Small Magellanic Cloud and the effect of metallicity on pulsation.
o	The EROS collaboration
o	Table 1: <[BKS97] NNNN> N=11 among (Nos 1448-9594)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKU2006]
[BKU2006]	(Bykov+Krassilchtchikov+Uvarov+, 2006) (Not yet in Simbad)
Write:	<<[BKU2006] CN>>
N:	4
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra sources in NGC 6334.
in source:	NGC 6334
Ref:	=2006A&A...449..917B
by	BYKOV A.M. , KRASSILCHTCHIKOV A.M., UVAROV Y.A., LEBRUN F., RENAUD M., TERRIER R., BLOEMEN H., McBREEN B., COURVOISIER T.J.-L., GUSTOV M.Y., HERMSEN W., LEYDER J.-C., LOZINSKAYA T.A., RAUW G., SWINGS J.-P.
	Astron. Astrophys., 449, 917-923 (2006)
	INTEGRAL detection of hard X-rays from NGC 6334: nonthermal emission from colliding winds or an AGN?
o	Fig.1b: <[BKU2006] CN> (Nos C1-C4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKU2008]
[BKU2008]	(Bykov+Krassilchtchikov+Uvarov+, 2008)
Write:	<<[BKU2008] Na>>
N:	3+2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton, Chandra, and Spitzer observations of IC 443.
in source:	IC 443
Ref:	=2008ApJ...676.1050B
by	BYKOV A.M. , KRASSILCHTCHIKOV A.M., UVAROV Y.A., BLOEMEN H., BOCCHINO F., DUBNER G.M., GIACANI E.B., PAVLOV G.G.
	Astrophys. J., 676, 1050-1063 (2008)
	Isolated X-Ray-Infrared sources in the region of interaction of the supernova remnant IC 443 with a molecular cloud.
o	Fig.2, Table 2: <[BKU2008] Na> (Nos 1-3, 1a, 1b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKU2016]
[BKU2016]	(Bresolin+Kudritzki+Urbaneja+, 2016)
Write:	<<[BKU2016] NN>>
N:	14
Object:	Poss. Blue Supergiant (SIMBAD class: BlueSG_Candidate = Blue Supergiant Candidate)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 observations of N=14 blue supergiant stars in M83. Use of archival HST WFC3 data. See also [BKU2022].
in source:	M 83 = NGC 5236
Ref:	=2016ApJ...830...64B
by	BRESOLIN F. , KUDRITZKI R.-P., URBANEJA M.A., GIEREN W., HO I.-T., PIETRZYNSKI G.
	Astrophys. J., 830, 64-64 (2016)
	Young stars and ionized nebulae in M83: comparing chemical abundances at high metallicity.
o	Table 1: <[BKU2016] NN> N=14.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKU2022]
[BKU2022]	(Bresolin+Kudritzki+Urbaneja, 2022)
Write:	<<[BKU2022] NN>>
N:	47
Object:	Poss. Blue Supergiant (SIMBAD class: BlueSG_Candidate = Blue Supergiant Candidate)
Note:	Keck I LRIS spectroscopy of N=47 blue supergiant candidates in NGC 2403. See also [BKU2016].
in source:	NGC 2403
Ref:	=2022ApJ...940...32B
by	BRESOLIN F. , KUDRITZKI R.-P., URBANEJA M.A.
	Astrophys. J., 940, 32 (2022)
	The Metallicity and Distance of NGC 2403 from Blue Supergiants.
o	Fig. 1, Table 1: <[BKU2022] NN> (Nos 1-47).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [BKV2009]
[BKV2009]	(Balog+Kiss+Vinko+, 2009)
Write:	<<[BKV2009] DDD.ddddd+DD.ddddd>> <<[BKV2009] NN>>
N:	201+19
Object:	* in Cl* (SIMBAD class: Star)
Note:	Spitzer/MIPS and IRAC observations, CTIO 1.5m photometry, and AAT spectroscopy of NGC 2451A and B.
in source:	NGC 2451
Ref:	=2009ApJ...698.1989B
by	BALOG Z. , KISS L.L., VINKO J., RIEKE G.H., MUZEROLLE J., GASPAR A., YOUNG E.T., GORLOVA N.
	Astrophys. J., 698, 1989-2013 (2009)
	Spitzer/IRAC-MIPS survey of NGC 2451A and B: debris disks at 50-80 million years.
o	Tables 3-6: <[BKV2009] DDD.ddddd+DD.ddddd> N=201. Figs 7+12, Table 7: <[BKV2009] NN> (Nos 1-19).
=E=	Catalogue in electronic form as <J/ApJ/698/1989/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BKV2013]
[BKV2013]	(Beygu+Kreckel+van de Weygaert+, 2013)
Write:	<<[BKV2013] VGS 31>> <<[BKV2013] VGS 31a>>
N:	1+3
Object:	Group of G + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	As part of the Void Galaxy Survey (VGS), study of a system (format VGS 31) of three interacting galaxies (format VGS 31a). See also [KPA2011].
Ref:	=2013AJ....145..120B
by	BEYGU B. , KRECKEL K., VAN DE WEYGAERT R., VAN DER HULST J.M., VAN GORKOM J.H.
	Astron. J., 145, 120 (2013)
	An interacting galaxy system along a filament in a void.
o	In this reference, VGS 31 is a galaxy group ([BKV2013] VGS 31), different from Kreckel et al. 2012 (2012AJ....144...16K, acronym [KPA2011]). Here, VGS 31a = [KPA2011] VGS 31 ; VGS 31b = [KPA2011] VGS 31a ; VGS 31c = [KPA2011] VGS 31b.
o	<[BKV2013] VGS 31> N=1. Fig. 1, Tables 2-5: <[BKV2013] VGS 31a> (Nos 31a-31c).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Bl
Bl	(Blanco)
*****	Avoid the usage of Bl, prefer [B61]
Details on Acronym: BL
BL	(Blair+Long)
*****	Avoid the usage of BL, prefer [BL2004b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BL
BL	(BL Lac Obj.)
*****	Avoid the usage of BL, prefer [HB93]
Details on Acronym: Bl
Bl	(Blanco)
Write:	<<PN Bl 1-A>> <<PN Bl 2-N>> <<PN Bl 3-NN>>
N:	17+1+14
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	List 1: format '1-A', N=17, (Nos A-Q). List 2: Bl 2-1 = PN G104.1+01.0 = PK 104+00 1. List 3: format '3-NN', 14 PN excerpted from a list of 22 objects.
in source:	NAME Gal Center
Ref:	=1961CoBos..13....1B
by	BLANCO V.M.
	Contr. from the Bosscha Observ. Lembang., 13, 1-11 (1961)
	A catalogue of Hα emission objects in the Galactic Center region.
o	<[B61] NN> (Nos 1-25). Table 2: <PN Bl 1-A> (Nos A-Q).
Details on Acronym: [BL2002]
[BL2002]	(Brodie+Larsen, 2002)
Write:	<<[BL2002] N1023-FF-NN>> <<[BL2002] N3384-FF-NN>>
N:	19+11
Object:	Poss. Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	Objects selected from HST WFPC2 data in NGC 1023 and NGC 3384 lenticular galaxies. Search for candidate stellar clusters. In the format 'FF' stands for 'Faint Fuzzies'. See also Paper I 2000AJ....120.2938L
in source:	NGC 1023
in source:	NGC 3384
Ref:	=2002AJ....124.1410B
by	BRODIE J.P. , LARSEN S.S.
	Astron. J., 124, 1410-1417 (2002)
	New members of the cluster family in nearby lenticular galaxies.
o	Table 1: <[BL2002] N1023-FF-NN> (Nos 1-19). Table 2: <[BL2002] N3384-FF-NN> (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BL2004]
[BL2004]	(Bouche+Lowenthal, 2004)= ([BL2004a])
Write:	<<[BL2004] QSO JHHMM+DDMM abs N.NNN>>
N:	2
Object:	DLA
Note:	N=1 DLA in PC 1233+4752 = QSO J1235+4736, already cited in White+ 1993ApJ...407..456W N=1 DLA in QSO J0124+0044, from Peroux, 2003, private comm.
Ref:	=2004ApJ...609..513B
by	BOUCHE N. , LOWENTHAL J.D.
	Astrophys. J., 609, 513-524 (2004)
	The clustering of galaxies around three z ~ 3 damped Lyα absorbers.
o	Table 1: DLA at z=2.974 in NAME APM 08279+5255 = QSO J0831+5245 is '[PAS2000] QSO J0831+5245 abs 2.974' in SIMBAD.
o	Table 1: <[BL2004] QSO J1235+4736 abs 3.499>, <[BL2004] QSO J0124+0044 abs 3.077>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BL2004a]
[BL2004a]	(Bouche+Lowenthal, 2004)
*****	Avoid the usage of [BL2004a], prefer [BL2004]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BL2004b]
[BL2004b]	(Blair+Long, 2004)= (BL)
Write:	<<[BL2004b] SNR NN>> <<[BL2004b] ONN>> <<[BL2004b] HII NN>>
N:	71+36+66
Object:	Poss. SNR + Nebula + HII (SIMBAD class: ISM = Interstellar Medium Object)
Note:	CTIO observations of M 83. N=71 SNR candidates are found, N=36 OIII:Halpha nebulae, N=66 HII regions.
in source:	M 83 = NGC 5236
Ref:	=2004ApJS..155..101B
by	BLAIR W.P. , LONG K.S.
	Astrophys. J., Suppl. Ser., 155, 101-121 (2004)
	An optical survey of supernova remnants in M 83.
o	Table 8: HII regions without coordinates, not in SIMBAD.
o	Table 5: <[BL2004b] SNR NN> (Nos 1-71). Table 6: <[BL2004b] ONN> (Nos O1-O36). Table 8: <[BL2004b] HII NN> (Nos 1-66).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BL2005]
[BL2005]	(Baek+Li, 2005)
Write:	<<[BL2005] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	KAIT images of UGC 11800: discovery of a variable star south of the nucleus.
Ref:	=2005IAUC.8574....2B
by	BAEK M. , LI W., (LOSS)
	IAU Circ., 8574, 2-None (2005)
	Variable stars near galaxies.
o	<[BL2005] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BL83]
[BL83]	(Bally+Lada, 1983)= (rho Oph)
Write:	<<[BL83] Rho Oph N>>
N:	5
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
in source:	NAME rho Oph Cloud
Ref:	=1983ApJ...265..824B
by	BALLY J. , LADA C.J.
	Astrophys. J., 265, 824-847 (1983)
	The high-velocity molecular flows near young stellar objects.
o	Tables 2, 3: <[BL83] Rho Oph N> (Nos 1-5)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BL86]
[BL86]	(Borra+Lepage, 1986)
Write:	<<[BL86] Star NN>> <<[BL86] QSO NN>>
N:	22+46
Object:	* + Poss. QSO (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table I: N=22 stars among (Nos 0-27), from calibrating sequence Table VI: N=46 QSO Candidates (Nos 1-46)
Ref:	=1986AJ.....92..203B
by	BORRA E.F. , LEPAGE R.
	Astron. J., 92, 203-212 (1986)
	Automated analysis of deep U, J and F plates: quasar and star counts past J = 22.
o	Coordinates of stars in plate 12 kindly provided by Brian Skiff.
o	Table I: <[BL86] Star NN> N=22 among (Nos 0-27), Table VI: <[BL86] QSO NN> (Nos 1-46)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BL97]
[BL97]	(Blair+Long, 1997)
Write:	<<[BL97] N300-ANN>> <<[BL97] N7793-ANN>> <<[BL97] N7793-S26ext>> <<[BL97] N7793-S26a>>
N:	28+28+4+22+22+11
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 3A: format 'N300-SNN', N=28 possible SNR in NGC 300 Table 3B: format 'N7793-SNN', N=28 possible SNR in NGC 7793 Table 3B, 5A: 'N7793-S26' is divided into 3 components '26a' to '26c' and has an exterior companion: '26ext' Table 4B: format 'N300-HNN', N=22 HII regions in NGC 300 Table 5B: format 'N7793-HNN', N=22 HII regions in NGC 7793 Table 5C: format 'N7793-DNN', N=11 Diffuse regions in NGC 7793 Maps and Identif. charts in Plates 3-26
in source:	NGC 300
in source:	NGC 7793
Ref:	=1997ApJS..108..261B
by	BLAIR W.P. , LONG K.S.
	Astrophys. J., Suppl. Ser., 108, 261-277 (1997)
	Identification of supernova remnants in the Sculptor group galaxies NGC 300 and NGC 7793.
o	Table 3A: <[BL97] N300-SNN> (Nos S1-S28). Tables 3B, 5A: <[BL97] N7793-SNN> (Nos S1-S28), <[BL97] N7793-S26ext> N=1, <[BL97] N7793-S26a> (Nos 26a-26c). Table 4B: <[BL97] N300-HNN> (Nos H1-H22). Table 5B: <[BL97] N7793-HNN> (Nos H1-H22). Table 5C: <[BL97] N7793-DNN> (Nos D11-D11)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BL98]
[BL98]	(Barvainis+Londsale, 1998) (Not yet in Simbad)
Write:	<<[BL98] OW 637 A>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Fig.4: (Nos A-D), 4 components of Ohio W 637.
in source:	OHIO W 637
Ref:	=1998AJ....115..885B
by	BARVAINIS R. , LONSDALE C.
	Astron. J., 115, 885-889 (1998)
	Search for free-free absorption cutoffs from tori in three type 2 active galactic nuclei.
o	Fig.4: <[BL98] OW 637 A> (Nos A-D)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Bla
Bla	(Blanco)
*****	Avoid the usage of Bla, prefer [B86]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Blanco
Blanco	(Blanco)
*****	Avoid the usage of Blanco, prefer [B62]
Details on Acronym: Blanco
Blanco	(Baade's window)
*****	Avoid the usage of Blanco, prefer [B84]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Blanco
Blanco	(Blanco)
Write:	<<Cl Blanco N>>
N:	1
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Stat:	is completely incorporated in Simbad
Ref:	=1949PASP...61..183B
by	BLANCO V.M.
	Publ. Astron. Soc. Pac., 61, 183-184 (1949)
	A new galactic star cluster in Sculptor.
o	<Cl Blanco 1> N=1
Details on Acronym: Blanco
Blanco	(Blanco)
*****	Avoid the usage of Blanco, prefer UBV
Details on Acronym: BLAST
BLAST	(Balloon-borne Large Aperture Submm Telescope) (Not yet in Simbad)
*****	Avoid the usage of BLAST, prefer [DAB2010]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BLAST
BLAST	(Balloon-borne Large Aperture Submm Telescope) (Not yet in Simbad)
====>	Equivalent to: [RAB2011b]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BLAST
BLAST	(Balloon-borne Large Aperture Submm Telescope)
Write:	<<BLAST JHHMMSS+DDMMSS>>
N:	60+69+79+76+15+1756+1440+1111+184
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	Balloon-borne Large Aperture Submillimeter Telescope (BLAST). 2008ApJ...681..428C: the BLAST survey in the Vulpecula region. See also [CAB2008]. 2009ApJ...707.1779E: the BLAST survey of the GOODS-South field. See also [ECD2009]. 2009Natur.458..737D: BLAST catalogs at 250, 350 nd 500µm. 2010ApJ...723..915R: the BLAST survey in the Aquila region. See also [RAB2010]. 2011ApJ...730..142R: the BLAST survey in the K3-50 and IC 5146 regions. See also [RAB2011]. 2011ApJ...727..114R: the BLAST survey in Cyg X. See also [RAB2011b]. 2009ApJ...707.1824N: the BLAST survey in the Vela region.
in source:	NAME Vulpecula Region
in source:	NAME GOODS South Field
in source:	NAME Aql Region
in source:	NAME Cyg X
in source:	NAME Vela Region
Ref:	=2008ApJ...681..428C
by	CHAPIN E.L. , ADE P.A.R., BOCK J.J., BRUNT C., DEVLIN M.J., DICKER S., GRIFFIN M., GUNDERSEN J.O., HALPERN M., HARGRAVE P.C., HUGHES D.H., KLEIN J., MARSDEN G., MARTIN P.G., MAUSKOPF P., NETTERFIELD C.B., OLMI L., PASCALE E., PATANCHON G., REX M., SCOTT D., SEMISCH C., TRUCH M.D.P., TUCKER C., TUCKER G.S., VIERO M.P., WIEBE D.V.
	Astrophys. J., 681, 428-452 (2008)
	The balloon-borne large aperture submillimeter telescope (BLAST) 2005: a 4 °^{2} galactic plane survey in Vulpecula (l = 59°).
o	Table 2, col(1): <[CAB2008] VNN> (Nos V01-V60) = Table 2, col(2): <BLAST JHHMMSS+DDMMSS> N=60.
Ref:	=2009ApJ...707.1779E
by	EALES S. , CHAPIN E.L., DEVLIN M.J., DYE S., HALPERN M., HUGHES D.H., MARSDEN G., MAUSKOPF P., MONCELSI L., NETTERFIELD C.B., PASCALE E., PATANCHON G., RAYMOND G., REX M., SCOTT D., SEMISCH C., SIANA B., TRUCH M.D.P., VIERO M.P.
	Astrophys. J., 707, 1779-1808 (2009)
	BLAST: the redshift survey.
o	Table 1: <[ECD2009] Rad DDD.ddddd+DD.ddddd>, <[ECD2009] IR DDD.ddddd+DD.ddddd>. Table 3: <[ECD2009] DD.ddddd+DD.ddddd> N=316.
Ref:	=2009ApJ...707.1824N
by	NETTERFIELD C.B. , ADE P.A.R., BOCK J.J., CHAPIN E.L., DEVLIN M.J., GRIFFIN M., GUNDERSEN J.O., HALPERN M., HARGRAVE P.C., HUGHES D.H., KLEIN J., MARSDEN G., MARTIN P.G., MAUSKOPF P., OLMI L., PASCALE E., PATANCHON G., REX M., ROY A., SCOTT D., SEMISCH C., THOMAS N., TRUCH M.D.P., TUCKER C., TUCKER G.S., VIERO M.P., WIEBE D.V.
	Astrophys. J., 707, 1824-1835 (2009)
	BLAST: the mass function, lifetimes, and properties of intermediate mass cores from a 50 °^{2} submillimeter galactic survey in Vela (l~265°).
o	Tables 1-2: <BLAST JHHMMSS+DDMMSS> N=1282.
Ref:	=2009Natur.458..737D
by	DEVLIN M.J. , ADE P.A.R., ARETXAGA I., BOCK J.J., CHAPIN E.L., GRIFFIN M., GUNDERSEN J.O., HALPERN M., HARGRAVE P.C., MARTIN P.G., MAUSKOPF P., MONCELSI L., NETTERFIELD C.B., NGO H., OLMI L., PASCALE E., PATANCHON G., REX M., SCOTT D., SEMISCH C., THOMAS N., TRUCH M.D.P., TUCKER C., TUCKER G.S., VIERO M.P., WIEBE D.
	Natur, 458, 737-739 (2009)
	Over half of the far-infrared background light comes from galaxies at z ~ 1.2.
o	Tables s2-s4: <BLAST JHHMMSS+DDMMSS> N=1756+1440+1111.
Ref:	=2010ApJ...723..915R
by	RIVERA-INGRAHAM A. , ADE P.A.R., BOCK J.J., CHAPIN E.L., DEVLIN M.J., DICKER S.R., GRIFFIN M., GUNDERSEN J.O., HALPERN M., HARGRAVE P.C., HUGHES D.H., KLEIN J., MARSDEN G., MARTIN P.G., MAUSKOPF P., NETTERFIELD C.B., OLMI L., PATANCHON G., REX M., SCOTT D., SEMISCH C., TRUCH M.D.P., TUCKER C., TUCKER G.S., VIERO M.P., WIEBE D.V.
	Astrophys. J., 723, 915-934 (2010)
	The BLAST view of the star-forming region in Aquila (l = 45°, b = 0°).
o	Table 1, col(1): <[RAB2010] ANNa> (Nos A0-A71, A28a, A30a, A53a, A59a) = Table 1, col(2): <BLAST JHHMMSS+DDMMSS> N=76. Table 2: <[RAB2010] ANNa-CNN> N=91. Fig. 14: <[RAB2010] GN> (Nos G1-G3).
Ref:	=2011ApJ...730..142R
by	ROY A. , ADE P.A.R., BOCK J.J., BRUNT C.M., CHAPIN E.L., DEVLIN M.J., DICKER S.R., FRANCE K., GIBB A.G., GRIFFIN M., GUNDERSEN J.O., HALPERN M., HARGRAVE P.C., HUGHES D.H., KLEIN J., MARSDEN G., MARTIN P.G., MAUSKOPF P., NETTERFIELD C.B., OLMI L., PATANCHON G., REX M., SCOTT D., SEMISCH C., TRUCH M.D.P., TUCKER C., TUCKER G.S., VIERO M.P., WIEBE D.V.
	Astrophys. J., 730, 142 (2011)
	Deconvolution of images from BLAST 2005: insight into the K3-50 and IC 5146 star-forming regions.
o	Table 1, col(1): <[RAB2011] KN> (Nos K1-K5) = Table 1, col(2): <BLAST JHHMMSS+DDMMSS> N=5. Table 2, col(1): <[RAB2011] ICNN> (Nos IC1-IC10) = Table 2, col(2): <BLAST JHHMMSS+DDMMSS> N=10. Fig. 10: <[RAB2011] GLL.ll+B.bb> N=3.
Ref:	=2011ApJ...727..114R
by	ROY A. , ADE P.A.R., BOCK J.J., CHAPIN E.L., DEVLIN M.J., DICKER S.R., FRANCE K., GIBB A.G., GRIFFIN M., GUNDERSEN J.O., HALPERN M., HARGRAVE P.C., HUGHES D.H., KLEIN J., MARSDEN G., MARTIN P.G., MAUSKOPF P., MORALES ORTIZ J.L., NETTERFIELD C.B., NORIEGA-CRESPO A., OLMI L., PATANCHON G., REX M., SCOTT D., SEMISCH C., TRUCH M.D.P., TUCKER C., TUCKER G.S., VIERO M.P., WIEBE D.V.
	Astrophys. J., 727, 114 (2011)
	The Balloon-borne Large Aperture Submillimeter Telescope (BLAST) 2005: a 10 °^{2} survey of star formation in Cygnus X.
o	Table 1, col(1): <[RAB2011b] CNNN> (Nos 0-183) = Table 1, col(2): <BLAST JHHMMSS+DDMMSS> N=184.
=E=	Catalogue in electronic form as <J/ApJ/681/428/>
=E=	Catalogue in electronic form as <J/ApJ/707/1779/>
=E=	Catalogue in electronic form as J/other/Nat/458.737
=E=	Catalogue in electronic form as <J/ApJ/723/915/>
=E=	Catalogue in electronic form as <J/ApJ/727/114/>
=E=	Catalogue in electronic form as <J/ApJ/707/1824/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BLAST
BLAST	(Balloon-borne Large Aperture Submm Telescope)
*****	Avoid the usage of BLAST, prefer [CAB2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BLAST
BLAST	(Balloon-borne Large Aperture Submilleter Telescope)
*****	Avoid the usage of BLAST, prefer [DAB2009]
Origin	of the Acronym: L (2009ApJ...707.1779E)
Details on Acronym: [BLB2003]
[BLB2003]	(Bik+Lamers+Bastian+, 2003)
Write:	<<[BLB2003] Cl NNN>> <<[BLB2003] HA NNN>>
N:	881+114
Object:	Cluster of * + Em.* (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST-WFPC2 observations of M 51. N=881 stellar clusters and N=114 H-alpha sources.
in source:	M 51
Ref:	=2003A&A...397..473B
by	BIK A. , LAMERS H.J.G.L.M., BASTIAN N., PANAGIA N., ROMANIELLO M.
	Astron. Astrophys., 397, 473-486 (2003)
	Clusters in the inner spiral arms of M51: The cluster IMF and the formation history.
o	Table 4: <[BLB2003] Cl NNN> (Nos 1-881). Table 5: <[BLB2003] HA NNN> (Nos 1-114).
=E=	Catalogue in electronic form as J/A+A/397/473
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLB2015]
[BLB2015]	(Bigiel+Leroy+Blitz+, 2015)
Write:	<<[BLB2015] N>>
N:	5
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	CARMA observations of the Antennae galaxies. Use of Herschel PACS data, part of the SHINING Survey.
in source:	NAME Antennae
Ref:	=2015ApJ...815..103B
by	BIGIEL F. , LEROY A.K., BLITZ L., BOLATTO A.D., DA CUNHA E., ROSOLOWSKY E., SANDSTROM K., USERO A.
	Astrophys. J., 815, 103 (2015)
	Dense gas fraction and star-formation efficiency variations in the Antennae galaxies.
o	Table 1: <[BLB2015] N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLB2018]
[BLB2018]	(Bellini+Libralato+Bedin+, 2018)
Write:	<<[BLB2018] NNNN>>
N:	5155
Object:	* (SIMBAD class: Star)
Note:	N=5155 stars in one of the parallel Hubble Space Telescope field, as part of the HST large programme on ω Centauri. See also [BAB2017] for stars in the core of ω Cen.
in source:	NGC 5139 = ome Cen
Ref:	=2018ApJ...853...86B
by	BELLINI A. , LIBRALATO M., BEDIN L.R., MILONE A.P., VAN DER MAREL R.P., ANDERSON J., APAI D., BURGASSER A.J., MARINO A.F., REES J.M.
	Astrophys. J., 853, 86-86 (2018)
	The HST large programme on ω Centauri. II. Internal kinematics.
o	Tables 4+6: <[BLB2018] NNNN> N=5155 among (Nos 48-5745).
=E=	Catalogue in electronic form as <J/ApJ/853/86/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLC2002]
[BLC2002]	(Berrington+Lugger+Cohn, 2002)
Write:	<<[BLC2002] NNNN>>
N:	319
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	WIYN Hydra Multi-Object spectrograph measures of ACO 2256.
in source:	ACO 2256
Ref:	=2002AJ....123.2261B
by	BERRINGTON R.C. , LUGGER P.M., COHN H.N.
	Astron. J., 123, 2261-2279 (2002)
	The dynamics of the merging galaxy cluster system A2256: evidence for a new subcluster.
o	AGK 224: not identified, incomplete format.
o	Table 3: <[BLC2002] NNNN> N=319 among (Nos 10-1080).
=E=	Catalogue in electronic form as J/AJ/123/2261
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLC2009]
[BLC2009]	(Bassani+Landi+Campana+, 2009)
Write:	<<[BLC2009] NN>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	N=2 Chandra sources near AX J183039-1002.
Ref:	=2009MNRAS.395L...1B
by	BASSANI L. , LANDI R., CAMPANA R., McBRIDE V.A., DEAN A.J., BIRD A.J., GREEN D.A., UBERTINI P., DE ROSA A.
	Mon. Not. R. Astron. Soc., 395L, 1-5 (2009)
	The nature of the ASCA/INTEGRAL source AX J183039-1002: a new Compton-thick AGN ?
o	Table 1: <[BLC2009] NN> (Nos N1-N2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLC99]
[BLC99]	(Boden+Lane+Creech-Eakman+, 1999) (Not yet in Simbad)
Write:	<<[BLC99] 64 Psc A>>
N:	2
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	64 Psc is a system with components A to C. N=2 apparent point sources in the field of 64 Psc, not companions of 64 PSc, (Nos D-E).
Ref:	=1999ApJ...527..360B
by	BODEN A.F. , LANE B.F., CREECH-EAKMAN M.J., COLAVITA M.M., DUMONT P.J., GUBLER J., KORESKO C.D., KUCHNER M.J., KULKARNI S.R., MOBLEY D.W., PAN X.P., SHAO M., VAN BELLE G.T., WALLACE J.K., OPPENHEIMER B.R.
	Astrophys. J., 527, 360-368 (1999)
	The visual orbit of 64 Piscium.
o	<[BLC99] 64 Psc A> (Nos D-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLD2000]
[BLD2000]	(Braine+Lisenfeld+Duc+, 2000)= (TDG)
Write:	<<[BLD2000] ANNNW>>
N:	2
Object:	Tidal dwarf G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=2 tidal dwarf galaxies related to APG 105 and APG 245 systems. See also [DBW97], [DBS2000], [BDL2001].
in source:	APG 105
in source:	APG 245
Ref:	=2000Natur.403..867B
by	BRAINE J. , LISENFELD U., DUC P.-A., LEON S.
	Nature, 403, 867-869 (2000)
	Formation of molecular gas in the tidal debris of violent galaxy-galaxy interactions.
o	(Erratum) erratum vol. 404 p.904 (2000)
o	Table 1: <[BLD2000] A105S> N=1, <[BLD2000] A245N> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLD2011]
[BLD2011]	(Buckley-Geer+Lin+Drabek+, 2011)
Write:	<<[BLD2011] galaxy>> <<[BLD2011] AN>> <<[BLD2011] NNNNN>>
N:	1+4+106
Object:	G + Grav. lensed image of a G (SIMBAD class: Galaxy)
Note:	Gemini South GMOS observations of a massive galaxy cluster (BCS J2352-5452 = SCSO J235138-545253).
Ref:	=2011ApJ...742...48B
by	BUCKLEY-GEER E.J. , LIN H., DRABEK E.R., ALLAM S.S., TUCKER D.L., ARMSTRONG R., BARKHOUSE W.A., BERTIN E., BRODWIN M., DESAI S., FRIEMAN J.A., HANSEN S.M., HIGH F.W., MOHR J.J., LIN Y.-T., NGEOW C.-C., REST A., SMITH R.C., SONG J., ZENTENO A.
	Astrophys. J., 742, 48 (2011)
	The serendipitous observation of a gravitationally lensed galaxy at z = 0.9057 from the Blanco Cosmology Survey: the Elliot Arc.
o	<[BLD2011] galaxy> N=1. Fig. 2, Table 2: <[BLD2011] AN> (Nos A1-A4). Tables 3-4: <[BLD2011] NNNNN> N=94+12 among (Nos 10692-19588).
=E=	Catalogue in electronic form as J/ApJ/742/48
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BlDz
BlDz	(Blaauw+Danziger+)= (BDS)
Write:	<<PN BlDz N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	BlDz 1 = PN G293.6+10.9 = PK 293+10 1
Ref:	=1975A&A....44..469B
by	BLAAUW A. , DANZIGER I.J., SCHUSTER H.E.
	Astron. Astrophys., 44, 469-471 (1975)
	A new southern planetary nebula.
o	<PN BlDz N> (No. 1).
Details on Acronym: [BLF2016]
[BLF2016]	(Basu-Zych+Lehmer+Fragos+, 2016)
Write:	<<[BLF2016] DD.ddddd+DD.ddddd>> <<[BLF2016] D.dddddd+DD.ddddd>>
N:	6+2
Object:	HMXB (SIMBAD class: HighMassXBin = High Mass X-ray Binary)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of N=6+2 high-mass X-ray binary (HMXB) sources in two Lyman break galaxies, VV 114 and Haro 11. Use archival of HST images.
in source:	VV 114
in source:	[H56] 11
Ref:	=2016ApJ...818..140B
by	BASU-ZYCH A.R. , LEHMER B., FRAGOS T., HORNSCHEMEIER A., YUKITA M., ZEZAS A., PTAK A.
	Astrophys. J., 818, 140 (2016)
	Exploring the overabundance of ULXs in metal- and dust-poor local Lyman break analogs.
o	Table 3: <[BLF2016] DD.ddddd+DD.ddddd> N=6, <[BLF2016] D.dddddd+DD.ddddd> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLF99]
[BLF99]	(Barkana+Lehar+Falco+, 1999) (Not yet in Simbad)
Write:	<<[BLF99] 0957+561 AN>>
N:	12
Object:	Component (SIMBAD class: Radio = Radio Source)
Note:	VLBI components of the double quasar QSO 0957+561A and B. See also YGKOW, [RGH85], [GWC92], [BTK93], [ACL97], [BFT97], [PMN99], [SOS99], [TF99].
in source:	QSO B0957+561
Ref:	=1999ApJ...520..479B
by	BARKANA R. , LEHAR J., FALCO E.E., GROGIN N.A., KEETON C.R., SHAPIRO I.I.
	Astrophys. J., 520, 479-490 (1999)
	A reassessment of the data and models of the gravitational lens Q0957+561.
o	Galaxy G1 = YGKOW G1
o	Table 1: <[BLF99] 0957+561 AN> (Nos A1-A6, B1-B6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BlFg
BlFg	(Blanco+Fitzgerald) (Not yet in Simbad)
*****	Avoid the usage of BlFg, prefer [BF64]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [BLH2002]
[BLH2002]	(Briceno+Luhman+Stauffer+, 2002)= (KPNO)
Write:	<<[BLH2002] KPNO-Tau NN>> <<[BLH2002] KPNO-Cand N>> <<[BLH2002] IRAS 04108+2803 A>>
N:	15+5+2
Object:	* (SIMBAD class: Star)
Note:	Search for low-mass Taurus members: N=15 new members, N=5 candidates. IRAS 04108+2803 YSO is a binary with 2 components A and B.
Ref:	=2002ApJ...580..317B
by	BRICENO C. , LUHMAN K.L., HARTMANN L., STAUFFER J.R., KIRKPATRICK J.D.
	Astrophys. J., 580, 317-335 (2002)
	The initial mass function in the Taurus star-forming region.
o	Parag. 4.2 : BR 2239-0447 is a misprint for 2339-0447
o	Table 2: <[BLH2002] KPNO-Tau N> (Nos 1-9). Table 3: <[BLH2002] KPNO-Cand N> (Nos 1-5). Table 5: <[BLH2002] IRAS 04108+2803 A> (Nos A-B).
Ref:	=2003ApJ...590..348L
by	LUHMAN K.L. , BRICENO C., STAUFFER J.R., HARTMANN L., BARRADO Y NAVASCUES D., CALDWELL N.
	Astrophys. J., 590, 348-356 (2003)
	New low-mass members of the Taurus star-forming region.
o	Table 2: <[BLH2002] KPNO-Tau NN> (Nos 10-15) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLH2011]
[BLH2011]	(Beuther+Linz+Henning+, 2011)
Write:	<<[BLH2011] N-NN>>
N:	73+44
Object:	smm Clump (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	APEX C18O(2-1) and 13CO(2-1) observations of the field of W 31. Use of 875µm data from the APEX ATLASGAL survey of the Galactic plane.
in source:	W 31
Ref:	=2011A&A...531A..26B
by	BEUTHER H. , LINZ H., HENNING Th., BIK A., WYROWSKI F., SCHULLER F., SCHILKE P., THORWIRTH S., KIM K.-T.
	Astron. Astrophys., 531A, 26-26 (2011)
	High-mass star formation at high luminosities: W31 at >10^{6} L_☉.
o	Tables 1-2: <[BLH2011] 1-NN> (Nos 1-73). Table 2: <[BLH2011] 2-NN> (Nos 1-44).
=E=	Catalogue in electronic form as J/A+A/531/A26
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLH2012]
[BLH2012]	(Beuther+Linz+Henning, 2012)
Write:	<<[BLH2012] 7538IRS1mm1>> <<[BLH2012] 7538SmmNa>>
N:	6 (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	Plateau de Bure Interferometer 1.36mm observations of the field of [WBN74] NGC 7538 IRS 1 and NGC 7538S.
Ref:	=2012A&A...543A..88B
by	BEUTHER H. , LINZ H., HENNING T.
	Astron. Astrophys., 543A, 88-88 (2012)
	The high-mass disk candidates NGC 7538 IRS 1 and NGC 7538S.
o	Table 2 : <[BLH2012] 7538IRS1mm1>, <[BLH2012] 7538SmmNa> (Nos Smm1-3, Smm1a, Smm1b)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLH97]
[BLH97]	(Bryce+Lopez+Holloway+, 1997) (Not yet in Simbad)
Write:	<<[BLH97] Knot NN>>
N:	19
Object:	Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=19 faint, irregular knots of emission observed ouside the main nebular structure of 'PN MyCn 18' Map Figs 1, 2, both refs.
Ref:	=1997ApJ...487L.161B
by	BRYCE M. , LOPEZ J.A., HOLLOWAY A.J., MEABURN J.
	Astrophys. J., 487, 161-164 (1997)
	A bipolar, knotty outflow with velocities of 500 kilometers per second from the engraved hourglass planetary nebula MyCn 18.
o	Table 1: <[BLH97] Knot NN> (Nos 1-14)
Ref:	=2000ApJ...531..336O
by	O'CONNOR J.A. , REDMAN M.P., HOLLOWAY A.J., BRYCE M., LOPEZ J.A., MEABURN J.
	Astrophys. J., 531, 336-344 (2000)
	The hypersonic, bipolar, knotty outflow from the engraved hourglass planetary nebula MyCn 18.
o	Fig.2, Table 2: <[BLH97] Knot NN> (Nos 15-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLI2003]
[BLI2003]	(Bolatto+Leroy+Israel+, 2003)= (MP) (Not yet in Simbad)
Write:	<<[BLI2003] MP NN>>
N:	14
Object:	CO peak (SIMBAD class: Cloud)
Note:	New CO observations of the LHA 115-N 83, 84 region of the SMC. 'MP' in the format stands for 'Molecular Peak'.
in source:	Magellanic Clouds:SMC:LHA 115-N 83 = LHA 115-N 83
in source:	Magellanic Clouds:SMC:LHA 115-N 84 = LHA 115-N 84
Ref:	=2003ApJ...595..167B
by	BOLATTO A.D. , LEROY A., ISRAEL F.P., JACKSON J.M.
	Astrophys. J., 595, 167-178 (2003)
	Unusual CO line ratios and kinematics in the N83/N84 region of the Small Magellanic Cloud.
o	Table 1: <[BLI2003] MP NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLK2010]
[BLK2010]	(Bonanos+Lennon+Kohlinger+, 2010)
Write:	<<[BLK2010] flamesNNNN>>
N:	134
Object:	* (SIMBAD class: Star)
Note:	VLT FLAMES observations of massive stars in the SMC.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2010AJ....140..416B
by	BONANOS A.Z. , LENNON D.J., KOHLINGER F., VAN LOON J.T., MASSA D.L., SEWILO M., EVANS C.J., PANAGIA N., BABLER B.L., BLOCK M., BRACKER S., ENGELBRACHT C.W., GORDON K.D., HORA J.L., INDEBETOUW R., MEADE M.R., MEIXNER M., MISSELT K.A., ROBITAILLE T.P., SHIAO B., WHITNEY B.A.
	Astron. J., 140, 416-429 (2010)
	Spitzer SAGE-SMC infrared photometry of massive stars in the Small Magellanic Cloud.
o	Tables 1, 3: <[BLK2010] flamesNNNN> N=134 among (Nos 1001-1246).
=E=	Catalogue in electronic form as J/AJ/140/416
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLK98]
[BLK98]	(Bershady+Lowenthal+Koo, 1998)
Write:	<<[BLK98] aa NNN>>
N:	116+14+50+35
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Keck telescope is used to count objects in the 2 fields 'SA 57' and Herc-1', centered respectively on '[K80] SA 57 6575' and '[K80] Herc-1 5677'.. There are 2 image classes j and k in each field, named 'sj' and 'sk' in SA 57 field, and 'hj' and 'hk' in Herc-1 field.
in source:	SA 57-
in source:	NAME Her 1
Ref:	=1998ApJ...505...50B
by	BERSHADY M.A. , LOWENTHAL J.D., KOO D.C.
	Astrophys. J., 505, 50-73 (1998)
	Near-infrared galaxy counts to J and K ~ 24 as a function of image size.
o	Table 2: <[BLK98] sk NNN> N=116, <[BLK98] sj NNN> N=14, <[BLK98] hk NNN> N=50, <[BLK98] hj NNN> N=35.
=E=	Catalogue in electronic form as J/ApJ/505/50
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLL2002]
[BLL2002]	(Beutler+Li+LOTOSS+, 2002)
Write:	<<[BLL2002] JHHMMSS.ss+DDMMSS.s>>
N:	2
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Stat:	is completely incorporated in Simbad
Note:	LOTOSS observations. Discovery of two new novae in M 31.
in source:	M 31 = NGC 224
Ref:	=2002IAUC.7937....3B
by	BEUTLER B. , LI W.D., LOTOSS
	IAU Circ., 7937, 3-None (2002)
	Novae in M31.
o	<[BLL2002] JHHMMSS.ss+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLL2005]
[BLL2005]	(Burket+Li+LOSS, 2005)
Write:	<<[BLL2005] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	KAIT observations. LOSS discovery of the apparent SN 2005AC 2".2 west and 0".9 south of the nucleus of of a compact galaxy.
Ref:	=2005IAUC.8478....2B
by	BURKET J. , LI W., (LOSS)
	IAU Circ., 8478, 2-None (2005)
	Supernova 2005ac.
o	<[BLL2005] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLL2010]
[BLL2010]	(Burningham+Leggett+Lucas+, 2010)
Write:	<<[BLL2010] SDSS J1416+13AB>> <<[BLL2010] SDSS J1416+13A>>
N:	1+2
Object:	** + in* (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	UKIRT WFCAM and Spitzer IRAC observations of a very cool common proper motion binary system. Use of UKIDSS LAS DR5 and SDSS DR7 data.
Ref:	=2010MNRAS.404.1952B
by	BURNINGHAM B. , LEGGETT S.K., LUCAS P.W., PINFIELD D.J., SMART R.L., DAY-JONES A.C., JONES H.R.A., MURRAY D., NICKSON E., TAMURA M., ZHANG Z., LODIEU N., TINNEY C.G., ZAPATERO OSORIO M.R.
	Mon. Not. R. Astron. Soc., 404, 1952-1961 (2010)
	The discovery of a very cool binary system.
o	Text: <[BLL2010] SDSS J1416+13AB> N=1, <[BLL2010] SDSS J1416+13A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLL93]
[BLL93]	(Bally+Lada+Lane, 1993) (Not yet in Simbad)
Write:	<<[BLL93] BN>> <<[BLL93] RN>>
N:	8
Object:	Bullet (SIMBAD class: PartofCloud = Part of Cloud)
Note:	N=4 CO bullets (Nos B1-B4) and N=4 SiO bullets (Nos R1-R4) in LDN 1448. See also [DDM94], [E2000].
in source:	LDN 1448
Ref:	=1993ApJ...418..322B
by	BALLY J. , LADA E.A., LANE A.P.
	Astrophys. J., 418, 322-327 (1993)
	The L 1448 molecular jet.
o	Fig.4: <[BLL93] AN> (Nos B1-B4, R1-R4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLM2007]
[BLM2007]	(Bassani+Landi+Malizia+, 2007)
Write:	<<[BLM2007] NN>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Swift XRT detection of N=2 sources inside the error box of IGR J22517+2218. Source N1 = IGR J22517+2218.
Ref:	=2007ApJ...669L...1B
by	BASSANI L. , LANDI R., MALIZIA A., FIOCCHI M.T., BAZZANO A., BIRD A.J., DEAN A.J., GEHRELS N., GIOMMI P., UBERTINI P.
	Astrophys. J., 669L, 1-4 (2007)
	IGR J22517+2218=MG3 J225155+2217: a new γ-ray lighthouse in the distant universe.
o	Table 1: <[BLM2007] AN> (Nos N1, N2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BLMC
BLMC	(Bright *)
Write:	<<BLMC NN>>
N:	20 among 55
Object:	Bright * (SIMBAD class: Star)
Note:	Table 1
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1987ApJ...321..156M
by	MOULD J. , REID N.
	Astrophys. J., 321, 156-161 (1987)
	The evolution of asymptotic giant branch stars in the Magellanic Clouds. III. The problem of intermediate-mass stars.
o	Table 1: <BLMC NN> N=20 among (Nos 1-55), Table 2: <CIII XNNN>, <CIII YNNN> and <CIII ZNNN> N=35
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BLO2005]
[BLO2005]	(Baum+Laor+O'Dea+, 2005) (Not yet in Simbad)
Write:	<<[BLO2005] NGC 1275 abs NN>>
N:	11
Object:	Absorber
Note:	HST STIS spectra of NGC 1275: absorption lines detected.
Ref:	=2005ApJ...632..122B
by	BAUM S.A. , LAOR A., O'DEA C.P., MACK J., KOEKEMOER A.M.
	Astrophys. J., 632, 122-136 (2005)
	Hubble Space Telescope STIS spectroscopy of the Lyα emission line in the central dominant galaxies in A426, A1795, and A2597: constraints on clouds in the intracluster medium.
o	Table 4: <[BLO2005] NGC 1275 abs NN> (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BLOX
BLOX	(Bonn Lensing, Optical, X-ray)
Write:	<<BLOX JHHMM.m+DDMM.m>>
N:	155
Object:	Poss. ClG (SIMBAD class: ClG_Candidate = Cluster of Galaxies Candidate)
Note:	Authors are conducting a wide-field imaging survey on deep, public XMM-Newton fields to carry out a combined search for galaxy clusters with weak gravitational lensing, optical and X-ray selection. If the three methods give different positions the "BLOX" name will be based on the most reliable position estimate.
Ref:	=2007A&A...470..821D
by	DIETRICH J.P. , ERBEN T., LAMER G., SCHNEIDER P., SCHWOPE A., HARTLAP J., MATURI M.
	Astron. Astrophys., 470, 821-834 (2007)
	BLOX: the Bonn lensing, optical, and X-ray selected galaxy clusters. I. Cluster catalog construction.
o	table1.dat: <BLOX JHHMM.m+DDMM.m> N=155.
=E=	Catalogue in electronic form as J/A+A/470/821
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [BLP2006]
[BLP2006]	(Baek+Li+Puckett+, 2006)
Write:	<<[BLP2006] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of SN 2006H.
Ref:	=2006IAUC.8660....1B
by	BAEK M. , LI W., PUCKETT T., SOSTERO G., GARZIA S.
	IAU Circ., 8660, 1-None (2006)
	Supernovae 2006D, 2006E, 2006F, 2006G, 2006H.
o	<[BLP2006] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLR2008]
[BLR2008]	(Bolatto+Leroy+Rosolowsky+, 2008)
Write:	<<[BLR2008] NGC NNNN NN>> <<[BLR2008] IC 10 NN>> <<[BLR2008] SMC LIRSNN N>> <<[BLR2008] SMC N83 N>> <<[BLR2008] LMC N159 N>> <<[BLR2008] MNN NN>>
N:	167
Object:	Giant MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	BIMA, OVRO, Plateau de Bure Interferometer, and SEST observations to search for giant molecular clouds in extragalactic systems.
Ref:	=2008ApJ...686..948B
by	BOLATTO A.D. , LEROY A.K., ROSOLOWSKY E., WALTER F., BLITZ L.
	Astrophys. J., 686, 948-965 (2008)
	The resolved properties of extragalactic giant molecular clouds.
o	Table 3: <[BLR2008] NGC NNNN NN>, <[BLR2008] IC 10 NN>, <[BLR2008] SMC LIRSNN N>, <[BLR2008] SMC N83 N>, <[BLR2008] LMC N159 N>, <[BLR2008] MNN NN>, N=172.
=E=	Catalogue in electronic form as <J/ApJ/686/948/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLR97]
[BLR97]	(Best+Longair+Rottgering, 1997)
Write:	<<[BLR97] 3C NNN.N a>> <<[BLR97] 3C NNN aW>> <<[BLR97] 3C NNN aa>> <<[BLR97] 3C NNN arc>>
N:	78
Object:	Component of rG (SIMBAD class: PartofG = Part of a Galaxy)
Note:	HST images of a sample of radio galaxies Fig.4 to Fig. 35: Maps of components in 20 radio galaxies
in source:	3C 13
in source:	3C 34
in source:	3C 41
in source:	3C 68.2
in source:	3C 217
in source:	3C 226
in source:	3C 239
in source:	3C 247
in source:	3C 265
in source:	3C 266
in source:	3C 280
in source:	3C 289
in source:	3C 324
in source:	3C 337
in source:	3C 340
in source:	3C 356
in source:	3C 368
in source:	3C 437
in source:	3C 441
in source:	3C 470
Ref:	=1997MNRAS.292..758B
by	BEST P.N. , LONGAIR M.S., ROETTGERING H.J.A.
	Mon. Not. R. Astron. Soc., 292, 758-794 (1997)
	HST, radio and infrared observations of 28 3CR radio galaxies at redshift z = 1 - I. The observations.
o	Fig.4 to Fig. 35: <[BLR97] 3C NNN a>, <[BLR97] 3C NNN.N a>, <[BLR97] 3C NNN aW>, <[BLR97] 3C NNN aa>, <[BLR97] 3C NNN arc>, N=78
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLS2007]
[BLS2007]	(Berta+Lonsdale+Siana+, 2007)
Write:	<<[BLS2007] LH-NNNNNN>> <<[BLS2007] EN1-NNNNNN>> <<[BLS2007] EN2-NNNNNN>>
N:	101+78+68
Object:	ULIRG (SIMBAD class: Galaxy)
Note:	Keck-LRIS optical spectroscopy of luminous galaxies in the SWIRE northern fields: Lockman Hole, ELAIS N1 and N2.
in source:	NAME Lockman Hole
in source:	ELAIS N1
in source:	ELAIS N2
Ref:	=2007A&A...467..565B
by	BERTA S. , LONSDALE C.J., SIANA B., FARRAH D., SMITH H.E., POLLETTA M.C., FRANCESCHINI A., FRITZ J., PEREZ-FOURNON I., ROWAN-ROBINSON M., SHUPE D., SURACE J.
	Astron. Astrophys., 467, 565-584 (2007)
	Keck spectroscopy of z = 1-3 ULIRGs from the Spitzer SWIRE survey.
o	Tables 5, 6: <[BLS2007] LH-NNNNNN> N=101, <[BLS2007] EN1-NNNNNN> N=78, <[BLS2007] EN2-NNNNNN> N=68.
=E=	Catalogue in electronic form as J/A+A/467/565
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLS87]
[BLS87]	(Bally+Langer+Stark+, 1987) (Not yet in Simbad)
Write:	<<[BLS87] NNa>>
N:	15
Object:	Clump (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Clumps in Ori A.
in source:	NAME Ori A
Ref:	=1987ApJ...312L..45B
by	BALLY J. , LANGER W.D., STARK A.A., WILSON R.W.
	Astrophys. J., 312, 45-49 (1987)
	Filamentary structure in the Orion molecular cloud.
o	Table 1: <[BLS87] NNa> (Nos 1-4, 5a-5b, 6-9, 10a-10b, 11a-11c).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLS90]
[BLS90]	(Braz+Lepine+Sivagnanam+, 1990)
Write:	<<[BLS90] HHMMm+DDMM>>
N:	9
Object:	OH Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	N=9 new OH masers associated with N=9 IRAS sources.
Ref:	=1990A&A...236..479B
by	BRAZ M.A. , LEPINE J.R.D., SIVAGNANAM P., LE SQUEREN A.M.
	Astron. Astrophys., 236, 479-486 (1990)
	New OH sources associated with young stellar objects.
o	Table 1: <[BLS90] HHMMm+DDMM> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLT2007]
[BLT2007]	(Burgarella+Le Floc'h+Takeuchi+, 2007)
Write:	<<[BLT2007] NNNNN>>
N:	45366
Object:	G (SIMBAD class: Galaxy)
Note:	Selection of UV galaxies from the GALEX survey.
Ref:	=2007MNRAS.380..986B
by	BURGARELLA D. , LE FLOC'H E., TAKEUCHI T.T., HUANG J.S., BUAT V., RIEKE G.H., TYLER K.D.
	Mon. Not. R. Astron. Soc., 380, 986-998 (2007)
	Lyman break galaxies at z ~ 1 and the evolution of dust attenuation in star-forming galaxies with redshift.
o	Table 1, col(2): <[BLT2007] NNNNN> (Nos 1-45366).
=E=	Catalogue in electronic form as J/MNRAS/380/986
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLT2013]
[BLT2013]	(Beuther+Linz+Tackenberg+, 2013)
Write:	<<[BLT2013] mmN>>
N:	4
Object:	Core (SIMBAD class: denseCore = Dense Core)
Note:	PdBI 93GHz observations of N=4 four sub-sources in the gas clump [BSM2002] 18310-0825 4.
in source:	[BSM2002] 18310-0825 4
Ref:	=2013A&A...553A.115B
by	BEUTHER H. , LINZ H., TACKENBERG J., HENNING T., KRAUSE O., RAGAN S., NIELBOCK M., LAUNHARDT R., BIHR S., SCHMIEDEKE A., SMITH R., SAKAI T.
	Astron. Astrophys., 553A, 115-115 (2013)
	Fragmentation and dynamical collapse of the starless high-mass star-forming region IRDC 18310-4.
o	Paragraph 4.2 G11.11 is probably GAL 011.11-00.12.
o	<NAME IRDC 18310-4>. Fig. 2, Table 2: <[BLT2013] mmN> (Nos mm1-mm4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLT2014]
[BLT2014]	(Beck+Lacy+Turner+, 2014)
Write:	<<[BLT2014] Central N>> <<[BLT2014] South N>> <<[BLT2014] W.Source>>
N:	7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 3.6cm continuum observations of N=7 radio sources in the nucleus of NGC 4194.
in source:	NGC 4194
Ref:	=2014ApJ...787...85B
by	BECK S.C. , LACY J., TURNER J., GREATHOUSE T., NEFF S.
	Astrophys. J., 787, 85 (2014)
	Ionized gas kinematics at high resolution. IV. Star formation and a rotating core in the Medusa (NGC 4194).
o	Table 2: <[BLT2014] South N> N=3, <[BLT2014] Central N> N=3, <[BLT2014] W.Source> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLV91]
[BLV91]	(Blair+Long+Vancura, 1991)
Write:	<<[BLV91] P2DiffN>> <<[BLV91] WWDN>>
N:	2+1
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	CCD imagery and spectrophotometry of Kepler's supernova remnant. P2Diff1 and P2Diff2 are two portions of the northeast difuse emission just northwest of the knot [DBD86] Knot 55. SWD9 is a previously uncatalogued knot 45" of [DBD86] Knot 9. See also [DBD86].
in source:	NAME Kepler SNR
Ref:	=1991ApJ...366..484B
by	BLAIR W. , LONG K.S., VANCURA O.
	Astrophys. J., 366, 484-494 (1991)
	A detailed optical study of Kepler's supernova remnant.
o	Table 2: knots DNN = [DBD86] Knot NN in Simbad.
o	Table 2: <[BLV91] P2Diff1>, <[BLV91] P2Diff2>, <[BLV91] SWD9>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BLW2004]
[BLW2004]	(Bremer+Lehnert+Waddington+, 2004)
Write:	<<[BLW2004] NN>>
N:	44
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Photometrically selected sample of candidate high-redshift galaxies from the HST ACS images of the CDFS (GOODS project).
in source:	NAME CDFS
Ref:	=2004MNRAS.347L...7B
by	BREMER M.N. , LEHNERT M.D., WADDINGTON I., HARDCASTLE M.J., BOYCE P.J., PHILLIPPS S.
	Mon. Not. R. Astron. Soc., 347, 7-12 (2004)
	The properties of Lyman break galaxies at z ~ 5.
o	Table 1: <[BLW2004] NN> (Nos 1-44).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BlX
BlX	(Blanco cluster, X-ray)
Write:	<<BlX NN>>
N:	88
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations of Cl Blanco 1
in source:	Cl Blanco 1
Ref:	=1999A&A...344...83M
by	MICELA G. , SCIORTINO S., FAVATA F., PALLAVICINI R., PYE J.
	Astron. Astrophys., 344, 83-96 (1999)
	X-ray observations of the young open cluster Blanco 1.
o	Table 2: objects 'NNN' = Cl* Blanco 1 ZS NNN, object W71 = Cl* Blanco 1 WGL 71.
o	Table 4: <BlX NN> (Nos 1-88).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BLZ2004]
[BLZ2004]	(Battz+Lauer+Zurek+, 2004)
Write:	<<[BLZ2004] PC1-N>> <<[BLZ2004] WFPC2-N>>
N:	7
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Search for microlensing candidates in M 87 with the WFPC2 instrument on the HST. N=7 variable sources, 4 are V*, 2 are consistent with classical novae, and one exhibit an excellent microlensing light curve.
in source:	M 87 = NGC 4486 = Virgo A
Ref:	=2004ApJ...610..691B
by	BALTZ E.A. , LAUER T.R., ZUREK D.R., GONDOLO P., SHARA M.M., SILK J., ZEPF S.E.
	Astrophys. J., 610, 691-706 (2004)
	Microlensing candidates in M87 and the Virgo cluster with the Hubble Space Telescope.
o	Table 2: <[BLZ2004] PC1-N> (Nos PC1-1 to 4), <[BLZ2004] WFPC2-N> (Nos WFPC2-5 to 7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BM
BM	(Blanco+Munch)= (TT)
Write:	<<BM R NNN>>
N:	542
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table IV: format 'IV NNN', (Nos 1-172), Carbon * Table V: format 'V NNN', (Nos 1-311), M * Table VI: format 'VI NN', (Nos 1-15), M supergiant * Table VII: format 'VII NN', (Nos 1-13), S * (often named TT in the literature) Table VIII: format 'VIII NN', (Nos 1-31), Stars with possible IR emission
Ref:	=1955BOTT....2l..17B
by	BLANCO V.M. , MUNCH L.
	Bol. Obs. Tonantz. Tacub., 2, part no 12, 17-29 (1955)
	Estrellas rojas entre Popa y Cruz.
o	Table IV: <BM IV NNN> (Nos 1-172). Table V: <BM V NNN> (Nos 1-311). Table VI: <BM VI NN> (Nos 1-15). Table VII: <BM VII NN> (Nos 1-13). Table VIII: <BM VIII NN> (Nos 1-31).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BM
BM	(Blanco+McCarthy)
*****	Avoid the usage of BM, prefer FBMC
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BM
BM	(Blanco+McCarthy)
*****	Avoid the usage of BM, prefer LMC-BM
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BM
BM	(Bidelman-MacConnell star)
*****	Avoid the usage of BM, prefer NBP
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BM2000]
[BM2000]	(Balogh+Morris, 2000)
Write:	<<[BM2000] xxxx.x+yyyy.y>>
N:	1189
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	ACO 2390
Ref:	=2000MNRAS.318..703B
by	BALOGH M.L. , MORRIS S.L.
	Mon. Not. R. Astron. Soc., 318, 703-714 (2000)
	Hα photometry of Abell 2390.
o	Table 2: ppp = CNOC ACO 2390 NNNNNN.
o	Table 2: <[BM2000] xxxx.x+yyyy.y> N=1189.
=E=	Catalogue in electronic form as J/MNRAS/318/703
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BM2003]
[BM2003]	(Buta+McCall, 2003)
Write:	<<[BM2003] NN>>
N:	20
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Stat:	is completely incorporated in Simbad
Note:	HST search for globular cluster candidates in Maffei 1.
in source:	Maffei 1
Ref:	=2003AJ....125.1150B
by	BUTA R. , McCALL M.L.
	Astron. J., 125, 1150-1163 (2003)
	Maffei 1 with the Hubble Space Telescope.
o	Table 3: <[BM2003] NN> (Nos 1-20).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BM2005]
[BM2005]	(Balland+Mouchet, 2005)
Write:	<<[BM2005] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of SN 1999GX.
Ref:	=2005IAUC.8517....1B
by	BALLAND C. , MOUCHET M.
	IAU Circ., 8517, 1-None (2005)
	Supernovae 1999gx and 2005bs.
o	<[BM2005] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BM54]
[BM54]	(Baade+Minkowski, 1954)
Write:	<<[BM54] Pup Na>> <<[BM54] Cas N>>
N:	8+3
Object:	Filament (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Fig. 9, Table 3: Filaments in Pup A SNR, (Nos 1-5, 6a-6b, 7) Fig. 3: Filaments in Cas A SNR, (Nos 1-3)
in source:	NAME Pup A
in source:	NAME Cas A
Ref:	=1954ApJ...119..206B
by	BAADE W. , MINKOWSKI R.
	Astrophys. J., 119, 206-214 (1954)
	Identification of the radio sources in Cassiopeia, Cygnus A, and Puppis A.
o	<[BM54] Pup Na> (Nos 1-5, 6a-6b, 7), <[BM54] Cas N> (Nos 1-3)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BM83]
[BM83]	(Bradt+McClintock, 1983)= (X)
Write:	<<[BM83] XHHMM+DDd>>
N:	127
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Table 1: Bright or compact discrete galactic X-ray sources N = 96 optical identifications Table 3: Bright source digest, N=115. Updates Bradt H.V.+, 1979, in X-ray Astronomy, ed Baity W.A., Peterson L.E., Oxford-Pergamon p. 3 (53 optical identif.)
Ref:	=1983ARA&A..21...13B
by	BRADT H.V.D. , McCLINTOCK J.E.
	Annual Rev. Astron. Astrophys., 21, 13-66 (1983)
	The optical counterparts of compact galactic X-ray sources.
o	Tables 1, 3: <[BM83] XHHMM+DDd> N=127.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BM89]
[BM89]	(Benson+Myers, 1989)
Write:	<<[BM89] N-NNN>> <<[BM89] 3A-NN>>
N:	119+30+5+10
Object:	Region (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	In the format, the first digit 'N' or 'NA' stands for the table number.
Ref:	=1989ApJS...71...89B
by	BENSON P.J. , MYERS P.C.
	Astrophys. J., Suppl. Ser., 71, 89-108 (1989)
	A survey for dense cores in dark clouds.
o	Table 1, col(2): MLB 3-NN. Table 2, col(2): MLB 4-NN (from 9 to 14, wrong cross-id. for N≥16).
o	Table 1: <[BM89] 1-NNN> (Nos 1-1 to 1-119). Table 2: <[BM89] 2-NN> (Nos 2-1 to 2-30), <MLB 4-NN> (Nos 4-21, 4-22) added. Table 3A: <[BM89] 3A-N> (Nos 3A-1 to 3A-5). Table 3B: <[BM89] 3B-NN> (Nos 3B-1 to 3B-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BM94]
[BM94]	(Belloni+Mereghetti, 1994)
Write:	<<[BM94] NN>>
N:	25
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	The 25 X-ray sources come from RX list.
in source:	RCW 49
Ref:	=1994A&A...286..935B
by	BELLONI T. , MEREGHETTI S.
	Astron. Astrophys., 286, 935-942 (1994)
	ROSAT observation of the giant HII region RCW 49.
o	<[BM94] NN> N=25
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BM98]
[BM98]	(Bennett+Moss, 1998)
Write:	<<[BM98] NN>>
N:	33
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	ACO 1060
Ref:	=1998A&AS..132...55B
by	BENNETT S.M. , MOSS C.
	Astron. Astrophys., Suppl. Ser., 132, 55-63 (1998)
	Hα objective prism survey of Abell 1060.
o	Table 3: <[BM98] NN> (Nos 1-33).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BM99]
[BM99]	(Brunzendorf+Meusinger, 1999)
Write:	<<[BM99] NNN>>
N:	660
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
in source:	ACO 426
Ref:	=1999A&AS..139..141B
by	BRUNZENDORF J. , MEUSINGER H.
	Astron. Astrophys., Suppl. Ser., 139, 141-161 (1999)
	The galaxy cluster Abell426 (Perseus). A catalogue of 660 galaxy positions, isophotal magnitudes and morphological types.
o	Catalog: <[BM99] NNN> (Nos 1-660).
=E=	Catalogue in electronic form as J/A+AS/139/141
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMA2003]
[BMA2003]	(Bahcall+McKay+Annis+, 2003)= (BH)
Write:	<<[BMA2003] BH NNN>>
N:	799
Object:	Cl of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	Catalog of 799 clusters in the redshift range 0.05-0.3 selected from SDSS data, using a color-magnitude red-sequence maxBCG technique (B) and a hybrid matched filter method (H).
Ref:	=2003ApJS..148..243B
by	BAHCALL N.A. , McKAY T.A., ANNIS J., KIM R.S.J., DONG F., HANSEN S., GOTO T., GUNN J.E., MILLER C., NICHOL R.C., POSTMAN M., SCHNEIDER D., SCHROEDER J., VOGES W., BRINKMANN J., FUKUGITA M.
	Astrophys. J., Suppl. Ser., 148, 243-274 (2003)
	A merged catalog of clusters of galaxies from early Sloan Digital Sky Survey data.
o	Table 2: <[BMA2003] BH NNN> (Nos 1-799).
=E=	Catalogue in electronic form as J/ApJS/148/243
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMA2005]
[BMA2005]	(Bamford+Milvang-Jensen+Aragon-Salamanca+, 2005)
Write:	<<[BMA2005] MSHHMM-NNNN>> <<[BMA2005] AC114-NNNN>> <<[BMA2005] A370-NNN>> <<[BMA2005] CL0054-NNNN>>
N:	17+14+18+33+11
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	VLT FORS2 observations of emission-line galaxies in clusters. Use of HST archival data.
in source:	1E 0440.5+0204 = ClG 0440+02
in source:	ACCG 114 = ACO S 1077
in source:	ACO 370
in source:	ClG 0054-27
in source:	1E 2053.7-0449 = ClG 2053-0449
Ref:	=2005MNRAS.361..109B
by	BAMFORD S.P. , MILVANG-JENSEN B., ARAGON-SALAMANCA A., SIMARD L.
	Mon. Not. R. Astron. Soc., 361, 109-127 (2005)
	The Tully-Fisher relation of distant cluster galaxies.
o	Table 3: objects in ClG 1054-03 are: format FNN = [MAH2003] FNN, format C01 = [MAH2003] C01, format NNNN = [VFK98] NNNN.
o	Table 3: <[BMA2005] MS0440-NNNN> N=17 among (Nos 101-1157), <[BMA2005] AC114-NNNN> N=14 among (Nos 18-1001), <[BMA2005] A370-NNN> N=18 among (Nos 39-751), <[BMA2005] CL0054-NNNN> N=33 among (Nos 62-1054), <[BMA2005] MS2053-NNNN> N=11 among (Nos 86-1296).
=E=	Catalogue in electronic form as J/MNRAS/361/109
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BMB
BMB	(Blanco+McCarthy+Blanco)
Write:	<<BMB NNN>>
N:	306
Object:	M Giant (SIMBAD class: AGB* = Asymptotic Giant Branch Star)
Stat:	is completely incorporated in Simbad
Note:	Late M giants found in Baade's Window Identif. charts
in source:	NGC 6522
Ref:	=1984AJ.....89..636B
by	BLANCO V.M. , McCARTHY M.F., BLANCO B.M.
	Astron. J., 89, 636-647 (1984)
	Giant M stars in Baade's Window.
o	Table I: <BMB NNN> (Nos 1-306)
=E=	Catalogue in electronic form as J/AJ/89/636
Details on Acronym: BMB-B
BMB-B	(Blanco+McCarthy+Blanco, Bar)= (SMC-B)
Write:	<<BMB-B NN>>
N:	83
Object:	Carbon and Late * (SIMBAD class: AGB* = Asymptotic Giant Branch Star)
Note:	Table 2, part A: (Nos 1-83), in the SMC Bar. Identif. charts.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1980ApJ...242..938B
by	BLANCO V.M. , McCARTHY M.F., BLANCO B.M.
	Astrophys. J., 242, 938-964 (1980)
	Carbon and late M-type stars in the Magellanic Clouds.
o	(misprint BMB-BW 66 =-69 not -59)
o	Table 2, part A: <BMB-B NN> (Nos 1-83), part B: <BMB-W NN> (Nos 1-56), part C: <BMB-BW NNN> (Nos 1-111), part D: <BMB-R NN> (Nos 1-61), part E: <BMB-O NNN> (Nos 1-116)
Details on Acronym: BMB-BW
BMB-BW	(Blanco+McCarthy+Blanco, Bar West)= (BW) = (LMC-BW)
Write:	<<BMB-BW NNN>>
N:	215+52
Object:	Carbon and Late * (SIMBAD class: AGB* = Asymptotic Giant Branch Star)
Note:	(Nos 1-215) and (Nos 301-352) Nos added in the 2nd ref. are based on an unpublished extension of the BMB survey. Identif. charts.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1980ApJ...242..938B
by	BLANCO V.M. , McCARTHY M.F., BLANCO B.M.
	Astrophys. J., 242, 938-964 (1980)
	Carbon and late M-type stars in the Magellanic Clouds.
o	(misprint BMB-BW 66 =-69 not -59)
o	Table 2, part A: <BMB-B NN> (Nos 1-83), part B: <BMB-W NN> (Nos 1-56), part C: <BMB-BW NNN> (Nos 1-111), part D: <BMB-R NN> (Nos 1-61), part E: <BMB-O NNN> (Nos 1-116)
Ref:	=1990ApJ...365..168F
by	FROGEL J.A. , BLANCO V.M.
	Astrophys. J., 365, 168-179 (1990)
	The Large Magellanic Cloud Bar West field.
o	Table 2: <BMB-BW NNN> (Nos 112-215) and (Nos 301-352) added
Details on Acronym: BMB-O
BMB-O	(Blanco+McCarthy+Blanco, Optical center)= (LMC-O)
Write:	<<BMB-O NNN>>
N:	116
Object:	Carbon and Late * (SIMBAD class: AGB* = Asymptotic Giant Branch Star)
Note:	Table 2, Part E: (Nos 1-116), in the LMC Optical center. Identif. charts
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1980ApJ...242..938B
by	BLANCO V.M. , McCARTHY M.F., BLANCO B.M.
	Astrophys. J., 242, 938-964 (1980)
	Carbon and late M-type stars in the Magellanic Clouds.
o	(misprint BMB-BW 66 =-69 not -59)
o	Table 2, part A: <BMB-B NN> (Nos 1-83), part B: <BMB-W NN> (Nos 1-56), part C: <BMB-BW NNN> (Nos 1-111), part D: <BMB-R NN> (Nos 1-61), part E: <BMB-O NNN> (Nos 1-116)
Details on Acronym: BMB-R
BMB-R	(Blanco+McCarthy+Blanco, Radio center)= (LMC-R)
Write:	<<BMB-R NN>>
N:	61
Object:	Carbon and Late * (SIMBAD class: AGB* = Asymptotic Giant Branch Star)
Note:	Table 2, part D: (Nos 1-61), in the LMC Radio center. Identif. charts
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1980ApJ...242..938B
by	BLANCO V.M. , McCARTHY M.F., BLANCO B.M.
	Astrophys. J., 242, 938-964 (1980)
	Carbon and late M-type stars in the Magellanic Clouds.
o	(misprint BMB-BW 66 =-69 not -59)
o	Table 2, part A: <BMB-B NN> (Nos 1-83), part B: <BMB-W NN> (Nos 1-56), part C: <BMB-BW NNN> (Nos 1-111), part D: <BMB-R NN> (Nos 1-61), part E: <BMB-O NNN> (Nos 1-116)
Details on Acronym: BMB-W
BMB-W	(Blanco+McCarthy+Blanco, Wing)= (SMC-W)
Write:	<<BMB-W NN>>
N:	56
Object:	Carbon and Late * (SIMBAD class: AGB* = Asymptotic Giant Branch Star)
Note:	Table 2, part B: (Nos 1-56), in the SMC Wing. Identif. charts
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1980ApJ...242..938B
by	BLANCO V.M. , McCARTHY M.F., BLANCO B.M.
	Astrophys. J., 242, 938-964 (1980)
	Carbon and late M-type stars in the Magellanic Clouds.
o	(misprint BMB-BW 66 =-69 not -59)
o	Table 2, part A: <BMB-B NN> (Nos 1-83), part B: <BMB-W NN> (Nos 1-56), part C: <BMB-BW NNN> (Nos 1-111), part D: <BMB-R NN> (Nos 1-61), part E: <BMB-O NNN> (Nos 1-116)
Details on Acronym: [BMB2007]
[BMB2007]	(Boyce+Myers+Browne+, 2007)
Write:	<<[BMB2007] J0316+4328 AN>>
N:	4+6
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	VLA, MERLIN, and VLBA observations of the lens system J0316+4328.
Ref:	=2007MNRAS.381L..55B
by	BOYCE E.R. , MYERS S.T., BROWNE I.W.A., STROMAN W.J., JACKSON N.J.
	Mon. Not. R. Astron. Soc., 381L, 55-59 (2007)
	J0316+4328: a probable `asymmetric double' lens.
o	In table 1 : J0316+3350 is a misprint for J0316+4328
o	Table 2, Figs 1-5, Paragr.3: <[BMB2007] J0316+4328 AN> (Nos A-D, A1-A3, B1-B3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMB2009]
[BMB2009]	(Burgess+Moraux+Bouvier+, 2009)= ([BMB2009a])
Write:	<<[BMB2009] IC348 CH4 N>>
N:	3
Object:	Poss. Brown Dwarf (SIMBAD class: BrownD*_Candidate = Brown Dwarf Candidate)
Stat:	is completely incorporated in Simbad
Note:	CFHT WIRCam and MegaCam observations of N=3 T-dwarf candidates in IC 348.
in source:	IC 348
Ref:	=2009A&A...508..823B
by	BURGESS A.S.M. , MORAUX E., BOUVIER J., MARMO C., ALBERT L., BOUY H.
	Astron. Astrophys., 508, 823-831 (2009)
	Young T-dwarf candidates in IC 348.
o	Tables 3-4: <[BMB2009] IC348 CH4 N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMB2009a]
[BMB2009a]	(Burgess+Moraux+Bouvier+, 2009)
*****	Avoid the usage of [BMB2009a], prefer [BMB2009]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMB2009b]
[BMB2009b]	(Bukowiecki+Maciejewski+Bykowski+, 2009)
Write:	<<[BMB2009b] VNN>>
N:	14
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	Rozhen National Astronomical Observatory 70-172cm Schmidt telescope observations of N=14 short-period variable stars in the field of NGC 957.
in source:	NGC 957
Ref:	=2009OEJV..112....1B
by	BUKOWIECKI L. , MACIEJEWSKI G., BYKOWSKI W., GEORGIEV T., BOEVA S., KACHAROV N., MIHOV B., LATEV G., OVCHAROV E., VALCHEVA A.
	OEJV, 112, 1 (2009)
	Search For Variable Stars in the Field of The Young Open Cluster NGC 957.
o	Table 1: <[BMB2009b] VNN> (Nos V1-V14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMB95]
[BMB95]	(Batuski+Maurogordato+Balkowski+, 1995)
Write:	<<[BMB95] ACO NNNN NN>>
N:	16+15+17+16+15
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Format 'ACO 2576 NN', N=16 G among 30 in ACO 2576 Format 'ACO 2628 NN', N=15 G among 25 in ACO 2628 Format 'ACO 3802 NN', N=17 G among 30 in ACO 3802 Format 'ACO 3817 NN', N=16 G among 30 in ACO 3817 Format 'ACO 3834 NN', N=15 G among 27 in ACO 3834
in source:	ACO 2576
in source:	ACO 2628
in source:	ACO 3802
in source:	ACO 3817
in source:	ACO 3834
Ref:	=1995A&A...294..677B
by	BATUSKI D.J. , MAUROGORDATO S., BALKOWSKI C., OLOWIN R.P.
	Astron. Astrophys., 294, 677-689 (1995)
	Redshift observations of Abell/ACO galaxy clusters in two candidate superclusters.
o	<[BMB95] ACO NNNN NN> N=16+15+17+16+15
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMB96]
[BMB96]	(Boselli+Mendes de Oliveira+Balkowski+, 1996)= (SCG)
Write:	<<[BMB96] N>>
N:	1
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	The authors found one new Southern Group of Galaxies
Ref:	=1996A&A...314..738B
by	BOSELLI A. , MENDES DE OLIVEIRA C., BALKOWSKI C., CAYATTE V., CASOLI F.
	Astron. Astrophys., 314, 738-744 (1996)
	The molecular gas content of spiral galaxies in compact groups.
o	<[BMB96] N> N=1. Table 1: <[BMB96] Na> (Nos 1a-1d)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMB96]
[BMB96]	(Boselli+Mendes de Oliveira+Balkowski+, 1996)= (SCG)
Write:	<<[BMB96] Na>>
N:	4
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
in source:	[BMB96] 1
Ref:	=1996A&A...314..738B
by	BOSELLI A. , MENDES DE OLIVEIRA C., BALKOWSKI C., CAYATTE V., CASOLI F.
	Astron. Astrophys., 314, 738-744 (1996)
	The molecular gas content of spiral galaxies in compact groups.
o	<[BMB96] N> N=1. Table 1: <[BMB96] Na> (Nos 1a-1d)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 1BMC
1BMC	(Brera Multi-scale wavelet Chandra survey)
Write:	<<1BMC JHHMMSS.s+DDMMSS>>
N:	21325
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	First Brera Multiscale Wavelet source catalog from Chandra ACIS-I images. See also [RCM2008].
Ref:	=2008A&A...488.1221R
by	ROMANO P. , CAMPANA S., MIGNANI R.P., MORETTI A., MOTTINI M., PANZERA M.R., TAGLIAFERRI G.
	Astron. Astrophys., 488, 1221-1236 (2008)
	The Brera multi-scale wavelet Chandra survey. I. Serendipitous source catalogue.
o	Catalog, col(1): <[RCM2008] NNNNN> (Nos 1-21325) = col(2): <1BMC JHHMMSS.s+DDMMSS> N=21325.
=E=	Catalogue in electronic form as J/A+A/488/1221
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BMC2009]
[BMC2009]	(Brown+Moustakas+Caldwell+, 2009)
Write:	<<[BMC2009] JHHMMSS.sss+DDMMSS.ss>>
N:	24
Object:	K+A galaxy (SIMBAD class: Galaxy)
Note:	MMT Hectospec observations of K+A galaxies from the AGN and Galaxy Evolution Survey.
in source:	NAME Bootes Field
Ref:	=2009ApJ...703..150B
by	BROWN M.J.I. , MOUSTAKAS J., CALDWELL N., PALAMARA D., COOL R.J., DEY A., HICKOX R.C., JANNUZI B.T., MURRAY S.S., ZARITSKY D.
	Astrophys. J., 703, 150-158 (2009)
	Active galactic nuclei and the truncation of star formation in K+A galaxies.
o	Table 1: <[BMC2009] JHHMMSS.sss+DDMMSS.ss> N=24.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMC2010]
[BMC2010]	(Bontemps+Motte+Csengeri+, 2010)
Write:	<<[BMC2010] CygX-NNN MMN>>
N:	24
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	IRAM PdBI 1.3 and 3.5mm observations towards the six most massive and youngest dense cores in the Cygnus X complex. See also [MBS2007c].
in source:	NAME CYG X: [MBS2007c] CygX-N3 = [MBS2007c] CygX-N3
in source:	NAME CYG X: [MBS2007c] CygX-N12 = [MBS2007c] CygX-N12
in source:	NAME CYG X: [MBS2007c] CygX-N40 = [MBS2007c] CygX-N40
in source:	NAME CYG X: [MBS2007c] CygX-N48 = [MBS2007c] CygX-N48
in source:	NAME CYG X: [MBS2007c] CygX-N53 = [MBS2007c] CygX-N53
in source:	NAME CYG X: [MBS2007c] CygX-N63 = [MBS2007c] CygX-N63
Ref:	=2010A&A...524A..18B
by	BONTEMPS S. , MOTTE F., CSENGERI T., SCHNEIDER N.
	Astron. Astrophys., 524A, 18-18 (2010)
	Fragmentation and mass segregation in the massive dense cores of Cygnus X.
o	Table 2: <[BMC2010] CygX-WNN MMN> N=24.
Details on Acronym: [BMC2017]
[BMC2017]	(Beifiori+Mendel+Chan+, 2017)
Write:	<<[BMC2017] XMM2215 NNNN>> <<[BMC2017] Cl0332 NNNNN>>
N:	46+17
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=46+17 passive galaxies in N=2 galaxy clusters at 1.39<z<1.61. Use of archival VLT K-band Multi-object Spectrograph (KMOS) Cluster Survey and HST images.
in source:	ClG J0332-2742
in source:	ClG J2215-1738
in source:	ClG J2235-2557
Ref:	=2017ApJ...846..120B
by	BEIFIORI A. , MENDEL J.T., CHAN J.C.C., SAGLIA R.P., BENDER R., CAPPELLARI M., DAVIES R.L., GALAMETZ A., HOUGHTON R.C.W., PRICHARD L.J., SMITH R., STOTT J.P., WILMAN D.J., LEWIS I.J., SHARPLES R., WEGNER M.
	Astrophys. J., 846, 120-120 (2017)
	The KMOS Cluster Survey (KCS). I. The fundamental plane and the formation ages of cluster galaxies at redshift 1.4 < z < 1.6.
o	Table 1: <[BMC2017] XMM2215 NNNN> N=6 among (Nos 615-1006), <[BMC2017] Cl0332 NNNNN> N=4 among (Nos 11827-25972).
Ref:	=2018ApJ...856....8C
by	CHAN J.C.C. , BEIFIORI A., SAGLIA R.P., MENDEL J.T., STOTT J.P., BENDER R., GALAMETZ A., WILMAN D.J., CAPPELLARI M., DAVIES R.L., HOUGHTON R.C.W., PRICHARD L.J., LEWIS I.J., SHARPLES R., WEGNER M.
	Astrophys. J., 856, 8-8 (2018)
	The KMOS Cluster Survey (KCS). II. The effect of environment on the structural properties of massive Cluster galaxies at redshift 1.39 < z < 1.61.
o	Table 11: <[BMC2017] XMM2215 NNNN> N=39 among (Nos 412-1261) added. Table 12: <[BMC2017] Cl0332 NNNNN> N=13 among (Nos 12347-25989) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMC2020]
[BMC2020]	(Beaklini+Mendoza+Canelo+, 2020)
Write:	<<[BMC2020] IRDC-C9 Main>> <<[BMC2020] IRDC-C9 Main Core>> <<[BMC2020] IRDC-C9 Main Tail>>
N:	1+1+1
Object:	(mm) + Dense Core (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=1 bright continuum source and N=2 substructures (Core and Tail in the formats) in the infrared dark cloud region [BT2009] C9, in archival ALMA Band 6 observations.
in source:	[BT2009] C9
Ref:	=2020MNRAS.491..427B
by	BEAKLINI P.P.B. , MENDOZA E., CANELO C.M., ALEMAN I., MERELLO M., KONG S., NAVARETE F., JANOT-PACHECO E., ABRAHAM Z., LEPINE J.R.D., DE ALMEIDA A.A., FRIACA A.C.S.
	Mon. Not. R. Astron. Soc., 491, 427-439 (2020)
	Sulphur-bearing and complex organic molecules in an infrared cold core.
o	Fig. 1: <[BMC2020] IRDC-C9 Main> N=1, <[BMC2020] IRDC-C9 Main Core> N=1, <[BMC2020] IRDC-C9 Main Tail> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMD2010]
[BMD2010]	(Badenes+Maoz+Draine, 2010)= (SNR)
Write:	<<[BMD2010] SNR JHHMM.m+DDMM>>
N:	77
Object:	SNR (SIMBAD class: SNRemnant = SuperNova Remnant)
Note:	N=77 SNRs in the Magellanic Clouds, from radio, optical, and X-ray SNR catalogs.
in source:	Magellanic Clouds:LMC = LMC
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2010MNRAS.407.1301B
by	BADENES C. , MAOZ D., DRAINE B.T.
	Mon. Not. R. Astron. Soc., 407, 1301-1313 (2010)
	On the size distribution of supernova remnants in the Magellanic clouds.
o	Table 1: <[BMD2010] SNR JHHMM.m+DDMM> N=77.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMD85]
[BMD85]	(Brown+Mundt+Drake, 1985)
Write:	<<[BMD85] FS Tau A>>
N:	2
Object:	* (SIMBAD class: Star)
Note:	N=2 stars near V* FS Tau (Haro 6-5). See also [MBF84].
Ref:	=1985ASSL..116..105B
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BME2006]
[BME2006]	(Bourke+Myers+Evans+, 2006)
Write:	<<[BME2006] L1521F-IRS>>
N:	1
Object:	Core (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC and MIPS observations of LDN 1521F.
in source:	LDN 1521F
Ref:	=2006ApJ...649L..37B
by	BOURKE T.L. , MYERS P.C., EVANS II N.J., DUNHAM M.M., KAUFFMANN J., SHIRLEY Y.L., CRAPSI A., YOUNG C.H., HUARD T.L., BROOKE T.Y., CHAPMAN N., CIEZA L., LEE C.W., TEUBEN P., WAHHAJ Z.
	Astrophys. J., 649, 37-40 (2006)
	The Spitzer c2d survey of nearby dense cores. II. Discovery of a low-luminosity object in the ``evolved starless core'' L1521F.
o	<[BME2006] L1521F-IRS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMF2001]
[BMF2001]	(Benedict+McArthur+Franz+, 2001) (Not yet in Simbad)
Write:	<<[BMF2001] Star N>>
N:	3
Object:	* (SIMBAD class: Star)
Note:	(Nos 2-4), reference stars in the field of Wolf 1062.
Ref:	=2001AJ....121.1607B
by	BENEDICT G.F. , McARTHUR B.E., FRANZ O.G., WASSERMAN L.H., HENRY T.J., TAKATO T., STRATEVA I.V., CRAWFORD J.L., IANNA P.A., McCARTHY D.W., NELAN E., JEFFERYS W.H., VAN ALTENA W., SHELUS P.J., HEMENWAY P.D., DUNCOMBE R.L., STORY D., WHIPPLE A.L., BRADLEY A.J., FREDRICK L.W.
	Astron. J., 121, 1607-1613 (2001)
	Precise masses for Wolf 1062 AB from Hubble Space Telescope interferometric astrometry and McDonald observatory radial velocities.
o	Table 2: <[BMF2001] Star N> (Nos 2-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMF2002]
[BMF2002]	(Benedict+McArthur+Fredrick+, 2002)= ([BMF2002a]) = (RR) (Not yet in Simbad)
Write:	<<[BMF2002] RR N>>
N:	5
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Note:	Reference stars for RR Lyr study.
Ref:	=2002AJ....123..473B
by	BENEDICT G.F. , McARTHUR B.E., FREDRICK L.W., HARRISON T.E., LEE J., SLESNICK C.L., RHEE J., PATTERSON R.J., NELAN E., JEFFERYS W.H., VAN ALTENA W., SHELUS P.J., FRANZ O.G., WASSERMAN L.H., HEMENWAY P.D., DUNCOMBE R.L., STORY D., WHIPPLE A.L., BRADLEY A.J.
	Astron. J., 123, 473-484 (2002)
	Astrometry with the Hubble Space Telescope: a parallax of the fundamental distance calibrator RR Lyrae.
o	Tables 3, 4: <[BMF2002] RR N> N=5 among (Nos 2-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMF2002a]
[BMF2002a]	(Benedict+McArthur+Fredrick+, 2002) (Not yet in Simbad)
*****	Avoid the usage of [BMF2002a], prefer [BMF2002]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMF2002b]
[BMF2002b]	(Benedict+McArthur+Fredrick+, 2002)= (DC)
Write:	<<[BMF2002b] DC N>>
N:	5
Object:	* (SIMBAD class: Star)
Note:	References stars for delta Cep (DC in the format).
Ref:	=2002AJ....124.1695B
by	BENEDICT G.F. , McARTHUR B.E., FREDRICK L.W., HARRISON T.E., SLESNICK C.L., RHEE J., PATTERSON R.J., SKRUTSKIE M.F., FRANZ O.G., WASSERMAN L.H., JEFFERYS W.H., NELAN E., VAN ALTENA W., SHELUS P.J., HEMENWAY P.D., DUNCOMBE R.L., STORY D., WHIPPLE A.L., BRADLEY A.J.
	Astron. J., 124, 1695-1705 (2002)
	Astrometry with the Hubble space telescope: a parallax of the fundamental distance calibrator δ Cephei.
o	Table 1, Fig.1: <[BMF2002b] DC N> (Nos 2-5, 7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMF2002c]
[BMF2002c]	(Benedict+McArthur+Forveille+, 2002) (Not yet in Simbad)
Write:	<<[BMF2002c] ref-N>>
N:	5
Object:	* (SIMBAD class: Star)
Note:	Reference stars. See also [BMF2003], [SNB2005].
Ref:	=2002ApJ...581L.115B
by	BENEDICT G.F. , McARTHUR B.E., FORVEILLE T., DELFOSSE X., NELAN E., BUTLER R.P., SPIESMAN W., MARCY G., GOLDMAN B., PERRIER C., JEFFERYS W.H., MAYOR M.
	Astrophys. J., 581, 115-118 (2002)
	A mass for the extrasolar planet Gliese 876b determined from Hubble Space Telescope fine guidance sensor 3 astrometry and high-precision radial velocities.
o	Tables 2, 3: <[BMF2002c] ref-N> (Nos 2-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMF2003]
[BMF2003]	(Benedict+McArthur+Fredrick+, 2003) (Not yet in Simbad)
Write:	<<[BMF2003] refN>>
N:	7
Object:	* (SIMBAD class: Star)
Note:	HST observations of PN NGC 6853 field. N=7 reference stars in that field. See also [BMF2002c], [SNB2005].
Ref:	=2003AJ....126.2549B
by	BENEDICT G.F. , McARTHUR B.E., FREDRICK L.W., HARRISON T.E., SKRUTSKIE M.F., SLESNICK C.L., RHEE J., PATTERSON R.J., NELAN E., JEFFERYS W.H., VAN ALTENA W., MONTEMAYOR T., SHELUS P.J., FRANZ O.G., WASSERMAN L.H., HEMENWAY P.D., DUNCOMBE R.L., STORY D., WHIPPLE A.L., BRADLEY A.J.
	Astron. J., 126, 2549-2556 (2003)
	Astrometry with the Hubble space telescope: a parallax of the central star of the planetary nebula NGC 6853.
o	Table 2: there is a misprint in Central Star (CS) coordinates, the central star of NGC 6853 could be 2MASS J19593637+2243159 or 2MASS J19593610+2243109.
o	Fig.1, Table 2: <[BMF2003] refN> (Nos ref2 to ref8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMF2009]
[BMF2009]	(Bortko+Martins+Fritz+, 2009) (Not yet in Simbad)
Write:	<<[BMF2009] NN>>
N:	90
Object:	* (SIMBAD class: Star)
Note:	VLT SINFONI and NOCA observations of N=90 W-R/O stars in the Galactic Center. See also [PGM2006].
in source:	NAME Gal Center
Ref:	=2009ApJ...697.1741B
by	BARTKO H. , MARTINS F., FRITZ T.K., GENZEL R., LEVIN Y., PERETS H.B., PAUMARD T., NAYAKSHIN S., GERHARD O., ALEXANDER T., DODDS-EDEN K., EISENHAUER F., GILLESSEN S., MASCETTI L., OTT T., PERRIN G., PFUHL O., REID M.J., ROUAN D., STERNBERG A., TRIPPE S.
	Astrophys. J., 697, 1741-1763 (2009)
	Evidence for warped disks of young stars in the Galactic Center.
o	Table 1: <[BMF2009] NN> (Nos 1-90).
=E=	Catalogue in electronic form as J/ApJ/697/1741
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMF2012]
[BMF2012]	(Beltran+Massi+Fontani+, 2012)
Write:	<<[BMF2012] source I>>
N:	1 (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	PdBI 2.7mm continuum observations of the region of IC 1396N.
Ref:	=2012A&A...542L..26B
by	BELTRAN M.T. , MASSI F., FONTANI F., CODELLA C., LOPEZ R.
	Astron. Astrophys., 542L, 26-26 (2012)
	Close encounters of the protostellar kind in IC 1396N.
o	Fig.2: <[BMF2012] source I>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BMG
BMG	(Bhatia+MacGillivray)
Write:	<<BMG NNN>>
N:	282
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1989A&A...211....9B
by	BHATIA R.K. , MacGILLIVRAY H.T.
	Astron. Astrophys., 211, 9-24 (1989)
	An automated search for star clusters in the Magellanic Clouds. I. Description of the technique and application to a 6 square ° field near the bear of the LMC.
o	Table 1: <BMG NNN> (Nos 1-282)
Details on Acronym: [BMG2009]
[BMG2009]	(Bernard+Monelli+Gallart+, 2009)
Write:	<<[BMG2009] Cetus ACS VNNN>> <<[BMG2009] Tucana VNNN>> <<[BMG2009] Cetus WFPC2 VNNN>>
N:	180+180+15
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	HST ACS and WFPC2 observations of Cetus and Tucana dwarf galaxies.
in source:	NAME Cetus Dwarf Galaxy
in source:	NAME Tucana Dwarf Galaxy
Ref:	=2009ApJ...699.1742B
by	BERNARD E.J. , MONELLI M., GALLART C., DROZDOVSKY I., STETSON P.B., APARICIO A., CASSISI S., MAYER L., COLE A.A., HIDALGO S.L., SKILLMAN E.D., TOLSTOY E.
	Astrophys. J., 699, 1742-1764 (2009)
	The ACS LCID project. I. Short-period variables in the isolated dwarf spheroidal galaxies Cetus and Tucana.
o	Table 7: <[BMG2009] Cetus ACS VNNN> (Nos V1-V180). Table 8: <[BMG2009] Tucana VNNN> (Nos V1-V371). Table 9: <[BMG2009] Cetus WFPC2 VNNN> (Nos V181-V195).
=E=	Catalogue in electronic form as <J/ApJ/699/1742/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMG2010]
[BMG2010]	(Bernard+Monelli+Gallart+, 2010)
Write:	<<[BMG2010] VNNN>> <<[BMG2010] VCNNN>>
N:	193+77
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations to search for variables in IC 1613.
in source:	IC 1613
Ref:	=2010ApJ...712.1259B
by	BERNARD E.J. , MONELLI M., GALLART C., APARICIO A., CASSISI S., DROZDOVSKY I., HIDALGO S.L., SKILLMAN E.D., STETSON P.B.
	Astrophys. J., 712, 1259-1276 (2010)
	The ACS LCID project. II. Faint variable stars in the isolated dwarf irregular galaxy IC 1613.
o	Finding chart.
o	Fig. 17, Tables 2-7: <[BMG2010] VNNN> (Nos V001-V193), <[BMG2010] VCNNN> (Nos VC194-VC270).
=E=	Catalogue in electronic form as <J/ApJ/712/1259/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMG2011]
[BMG2011]	(Bannister+Murphy+Gaensler+, 2011)
Write:	<<[BMG2011] JHHMMSS+DDMMSS>>
N:	7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=7 transient radio sources found in archival images taken with the Molonglo Observatory Synthesis Telescope (MOST).
Ref:	=2011MNRAS.412..634B
by	BANNISTER K.W. , MURPHY T., GAENSLER B.M., HUNSTEAD R.W., CHATTERJEE S.
	Mon. Not. R. Astron. Soc., 412, 634-664 (2011)
	A 22-yr southern sky survey for transient and variable radio sources using the Molonglo Observatory Synthesis Telescope.
o	(Erratum) erratum vol. 418, p.2813 (2011)
o	Tables 6-7: <[BMG2011] JHHMMSS+DDMMSS> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMG2013]
[BMG2013]	(Bernard+Monelli+Gallart+, 2013)
Write:	<<[BMG2013] VNNN>> <<[BMG2013] VCNN>>
N:	166+33
Object:	V* + Poss. V* (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations of N=166 variable stars and N=33 candidate variables in Leo 2 galaxy. See also [DSC2002] and [HSK94].
in source:	NAME Leo A
Ref:	=2013MNRAS.432.3047B
by	BERNARD E.J. , MONELLI M., GALLART C., FIORENTINO G., CASSISI S., APARICIO A., COLE A.A., DROZDOVSKY I., HIDALGO S.L., SKILLMAN E.D., STETSON P.B., TOLSTOY E.
	Mon. Not. R. Astron. Soc., 432, 3047-3061 (2013)
	The ACS LCID project - VIII. The short-period cepheids of Leo A.
o	Table 3: <[BMG2013] VNNN> (Nos 1-166). Table 4: <[BMG2013] VCNN> (Nos 1-33)>.
=E=	Catalogue in electronic form as <J/MNRAS/432/3047/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMG2016]
[BMG2016]	(Belloche+Mueller+Garrod+, 2016)
Write:	<<[BMG2016] Sgr B2(NN)>>
N:	5
Object:	mm core (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	ALMA 3mm observations of N=5 hot cores in Sgr B2(N).
in source:	NAME SGR B2:NAME SGR B2(N) = NAME SGR B2(N)
Ref:	=2016A&A...587A..91B
by	BELLOCHE A. , MUELLER H.S.P., GARROD R.T., MENTEN K.M.
	Astron. Astrophys., 587A, 91-91 (2016)
	Exploring molecular complexity with ALMA (EMoCA): Deuterated complex organic molecules in Sagittarius B2(N2).
o	<[BMG2016] Sgr B2(NN)> (Nos N1-N2).
Ref:	=2017A&A...604A..60B
by	BONFAND M. , BELLOCHE A., MENTEN K.M., GARROD R.T., MUELLER H.S.P.
	Astron. Astrophys., 604A, 60-60 (2017)
	Exploring molecular complexity with ALMA (EMoCA): Detection of three new hot cores in Sagittarius B2(N).
o	Fig. 2, Table 1: <[BMG2016] Sgr B2(NN)> (Nos N3-N5) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMG2017]
[BMG2017]	(Bhattacharya+Mohana+Gulati+, 2017)
Write:	<<[BMG2017] 3EG JHHMM+DDMM newN>>
N:	39
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	N=39 gamma-ray sources in the field of 10 EGRET sources. Use of Fermi data.
Ref:	=2017MNRAS.471.5008B
by	BHATTACHARYA D. , MOHANA K.A., GULATI S., BHATTACHARYYA S., BHATT N., SREEKUMAR P., STALIN C.S.
	Mon. Not. R. Astron. Soc., 471, 5008-5017 (2017)
	Unusual long-term low-activity states of EGRET blazars in the Fermi era.
o	Table 3: <[BMG2017] 3EG JHHMM+DDMM newN> N=39.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMH2001]
[BMH2001]	(Barris+Miknaitis+High Z supernova search team+, 2001)
Write:	<<[BMH2001] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host G of SN 2001GA.
Ref:	=2001IAUC.7755....2B
by	BARRIS B. , MIKNAITIS G., (The High-Z Supernova Search Team), GARNAVICH P., QUINN J., CHALLIS P., MARTIN E., FILIPPENKO A.V., CHORNOCK R.
	IAU Circ., 7755, 2-None (2001)
	Supernova 2001ga in anonymous galaxy.
o	<[BMH2001] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMH2011]
[BMH2011]	(Bellagamba+Maturi+Hamana+, 2011)
Write:	<<[BMH2011] NNN>>
N:	147
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	Search for galaxy clusters in the COSMOS field.
in source:	NAME COSMOS Field
Ref:	=2011MNRAS.413.1145B
by	BELLAGAMBA F. , MATURI M., HAMANA T., MENEGHETTI M., MIYAZAKI S., MOSCARDINI L.
	Mon. Not. R. Astron. Soc., 413, 1145-1157 (2011)
	Optimal filtering of optical and weak lensing data to search for galaxy clusters: application to the COSMOS field.
o	Tables 1, A1: <[BMH2011] NNN> (Nos 1-147).
=E=	Catalogue in electronic form as <J/MNRAS/413/1145/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMH2014]
[BMH2014]	(Broekhoven-Fiene+Matthews+Harvey+, 2014)
Write:	<<[BMH2014] NNN>> <<[BMH2014] Group N>>
N:	166+7
Object:	YSO + Poss. YSO + Cluster of * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Spitzer (IRAC and MIPS) and WISE observations of the Auriga-California Molecular Cloud as part of the Spitzer Gould Belt Legacy Survey. See also SSTgbs.
in source:	Gould Belt:NAME Auriga-California Molecular Cloud = NAME Auriga-California Molecular Cloud
Ref:	=2014ApJ...786...37B
by	BROEKHOVEN-FIENE H. , MATTHEWS B.C., HARVEY P.M., GUTERMUTH R.A., HUARD T.L., TOTHILL N.F.H., NUTTER D., BOURKE T.L., DIFRANCESCO J., JORGENSEN J.K., ALLEN L.E., CHAPMAN N.L., CIEZA L.A., DUNHAM M.M., MERIN B., MILLER J.F., TEREBEY S., PETERSON D.E., STAPELFELDT K.R.
	Astrophys. J., 786, 37 (2014)
	The Spitzer survey of interstellar clouds in the Gould belt. VI. The Auriga-California molecular cloud observed with IRAC and MIPS.
o	(Erratum) erratum vol. 798, art. 65 (2015)
o	Tables 4-5, col(1): <[BMH2014] NNN> (Nos 1-166) = Tables 4-5, col(2): <SSTgbs JHHMMSSss+DDMMSSs> N=166. Table 9: <[BMH2014] Group N> (Nos 1-7).
=E=	Catalogue in electronic form as <J/ApJ/786/37/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMK2001]
[BMK2001]	(Blakeslee+Metzger+Kuntschner+, 2001)= ([BMK2001a])
Write:	<<[BMK2001] A>> <<[BMK2001] GN>>
N:	1+3
Object:	Arc + G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck observations of Hercules cluster = ACO 2151: The finding chart of ACO 2151 includes an arclet 'A' (lens model) and 3 early-type galaxies (Nos G1-G3).
Ref:	=2001AJ....121....1B
by	BLAKESLEE J.P. , METZGER M.R., KUNTSCHNER H., COTE P.
	Astron. J., 121, 1-9 (2001)
	Lensing in the Hercules supercluster.
o	UGC 10187 NED 01 and NED 02 are respectively MCG+03-41-094 = NAME ACO 2152 SRG in SIMBAD, and MCG+03-41-095 = NAME ACO 2152 BCG in SIMBAD. Galaxy M in fig.1 = [BH98] 16031+1633 .
o	Fig.1, Table 1: <[BMK2001] A> (No. A), <[BMK2001] GN> (Nos G1-G3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMK2001a]
[BMK2001a]	(Blakeslee+Metzger+Kuntschner+, 2001)
*****	Avoid the usage of [BMK2001a], prefer [BMK2001]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMK2001b]
[BMK2001b]	(Boyce+Minchin+Kilborn+, 2001)= (HIJASS)
Write:	<<[BMK2001b] HIJASS JHHMM+DDMM>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
in source:	NAME M 81 GROUP
Ref:	=2001ApJ...560L.127B
by	BOYCE P.J. , MINCHIN R.F., KILBORN V.A., DISNEY M.J., LANG R.H., JORDAN C.A., GROSSI M., LYNE A.G., COHEN R.J., MORISON I.M., PHILLIPPS S.
	Astrophys. J., 560, 127-130 (2001)
	A blind H I survey of the M81 group.
o	Fig.2: Features = [ADS81] VI and VIII.
o	<[BMK2001b] HIJASS JHHMM+DDMM> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMK2014]
[BMK2014]	(Bell+Murphy+Kaplan+, 2014) (Not yet in Simbad)
Write:	<<[BMK2014] MWA JHHMM+DDMM>>
N:	6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Murchison Widefield Array (MWA) 154MHz observations of N=6 variable radio sources.
Ref:	=2014MNRAS.438..352B
by	BELL M.E. , MURPHY T., KAPLAN D.L., HANCOCK P., GAENSLER B.M., BANYER J., BANNISTER K., TROTT C., HURLEY-WALKER N., WAYTH R.B., MacQUART J.-P., ARCUS W., BARNES D., BERNARDI G., BOWMAN J.D., BRIGGS F., BUNTON J.D., CAPPALLO R.J., COREY B.E., DESHPANDE A., DESOUZA L., EMRICH D., GOEKE R., GREENHILL L.J., HAZELTON B.J., HERNE D., HEWITT J.N., JOHNSTON-HOLLITT M., KASPER J.C., KINCAID B.B., KOENIG R., KRATZENBERG E., LONSDALE C.J., LYNCH M.J., McWHIRTER S.R., MITCHELL D.A., MORALES M.F., MORGAN E., OBEROI D., ORD S.M., PATHIKULANGARA J., PRABU T., REMILLARD R.A., ROGERS A.E.E., ROSHI A., SALAH J.E., SAULT R.J., UDAYA SHANKAR N., SRIVANI K.S., STEVENS J., SUBRAHMANYAN R., TINGAY S.J., WATERSON M., WEBSTER R.L., WHITNEY A.R., WILLIAMS A., WILLIAMS C.L., WYITHE J.S.B.
	Mon. Not. R. Astron. Soc., 438, 352-367 (2014)
	A survey for transients and variables with the Murchison Widefield Array 32-tile prototype at 154MHz.
o	Tables 3+5: <[BMK2014] MWA JHHMM+DDMM> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BML
BML	(Broad Molecular Line)
*****	Avoid the usage of BML, prefer [RRJ2005]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BML2002]
[BML2002]	(Busarello+Merluzzi+La Barbera+, 2002)
Write:	<<[BML2002] NNNN>>
N:	1206
Object:	* + G in ClG (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	EMMI ESO NTT observations. Photometric data in the field of ACCG 118.
in source:	ACCG 118 = ACO 2744
Ref:	=2002A&A...389..787B
by	BUSARELLO G. , MERLUZZI P., LA BARBERA F., MASSAROTTI M., CAPACCIOLI M.
	Astron. Astrophys., 389, 787-794 (2002)
	Optical (VRI) photometry in the field of the galaxy cluster AC118 at z=0.31.
o	Table 3: <[BML2002] NNNN> (Nos 1-1206).
=E=	Catalogue in electronic form as J/A+A/389/787
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BML2009]
[BML2009]	(Beltran+Massi+Lopez+, 2009)
Write:	<<[BML2009] NIR NNNNA>> <<[BML2009] ANN>>
N:	736+88
Object:	(NIR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	TNG NICS observations of the IC 1396N region in the JHK' (broadband) and H2 (narrowband) filters.
in source:	IC 1396N
Ref:	=2009A&A...504...97B
by	BELTRAN M.T. , MASSI F., LOPEZ R., GIRART J.M., ESTALELLA R.
	Astron. Astrophys., 504, 97-107 (2009)
	The stellar population and complex structure of the bright-rimmed cloud IC 1396N.
o	Tables 1-4: <[BML2009] NIR NNNNA> N=736. Table 5: <[NMV2001] Knot A> (Nos T-V) added, <[BML2009] ANN> N=88.
=E=	Catalogue in electronic form as J/A+A/504/97
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BML2014]
[BML2014]	(Bruursema+Meixner+Long+, 2014)
Write:	<<[BML2014] NN>>
N:	48
Object:	Poss. SNR (SIMBAD class: SNRemnant_Candidate = SuperNova Remnant Candidate)
Note:	WIYN 3.5-m telescope High Resolution Infrared Camera (WHIRC) JH and narrowband observations of N=48 SNR candidates in NGC 6946.
in source:	NGC 6946
Ref:	=2014AJ....148...41B
by	BRUURSEMA J. , MEIXNER M., LONG K.S., OTSUKA M.
	Astron. J., 148, 41 (2014)
	A search for supernova remnants in NGC 6946 using the [Fe II] 1.64 µm line.
o	Fig. 3, Table 4: <[BML2014] NN> (Nos 1-48).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BMLH2
BMLH2	(Broad Molecular Line, H2)
Write:	<<BMLH2 NN>>
N:	16
Object:	H2 Clump (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=16 H2 clumps in the nebula NAME 3C 391 BML
in source:	3C 391:NAME 3C 391 BML = NAME 3C 391 BML
Ref:	=2002ApJ...564..302R
by	REACH W.T. , RHO J., JARRETT T.H., LAGAGE P.-O.
	Astrophys. J., 564, 302-316 (2002)
	Molecular and ionic shocks in the supernova remnant 3C 391.
o	Table 3: <BMLH2 NN> (Nos 1-12).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BMM2000]
[BMM2000]	(Belczynski+Mikolajewska+Munari+, 2000) (Not yet in Simbad)
Write:	<<[BMM2000] NNN>> <<[BMM2000] sNN>>
N:	188+30
Object:	Sy* (SIMBAD class: Symbiotic* = Symbiotic Star)
Note:	Table 1: N=188 symbiotic stars. Table 2: N=30 suspected symbiotic stars.
Ref:	=2000A&AS..146..407B
by	BELCZYNSKI K. , MIKOLAJEWSKA J., MUNARI U., IVISON R.J., FRIEDJUNG M.
	Astron. Astrophys., Suppl. Ser., 146, 407-435 (2000)
	A catalogue of symbiotic stars.
o	Table 1: <[BMM2000] NNN> (Nos 1-188). Table 2: <[BMM2000] sNN> (Nos s01-s30).
=E=	Catalogue in electronic form as J/A+AS/146/407
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMM2010]
[BMM2010]	(Brink+Mateo+Martinez-Delgado, 2010)
Write:	<<[BMM2010] NNNNNN>> <<[BMM2010] NNNNN>>
N:	328+272
Object:	* (SIMBAD class: Star)
Note:	INT WFC imaging and 6.5m Baade telescope IMACS spectroscopy of a field centered on the Virgo Stellar Stream at (RA, DE)~(185.9deg, -1.0deg), and of a control field centered at (RA, DE)~(228.5deg, 9.9deg). Format NNNNNN: N=328 stars in the Virgo field. Format NNNNN: N=272 stars in the control field.
Ref:	=2010AJ....140.1337B
by	BRINK T.G. , MATEO M., MARTINEZ-DELGADO D.
	Astron. J., 140, 1337-1346 (2010)
	Radial velocities of Galactic halo stars in Virgo.
o	Table 1: <[BMM2010] NNNNNN> N=328 among (Nos 103180-403879). Table 2: <[BMM2010] NNNNN> N=272 among (Nos 11205-40960).
=E=	Catalogue in electronic form as <J/AJ/140/1337/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMM2014]
[BMM2014]	(Balogh+Mcgee+Mok+, 2014)
Write:	<<[BMM2014] NNNNNNN>>
N:	9245
Object:	G (SIMBAD class: Galaxy)
Note:	Gemini South GMOS spectroscopy of N=9245 galaxies in the fields of 11 galaxy groups within the COSMOS field. See also [GSF2010] for the galaxy groups.
Ref:	=2014MNRAS.443.2679B
by	BALOGH M.L. , McGEE S.L., MOK A., WILMAN D.J., FINOGUENOV A., BOWER R.G., MULCHAEY J.S., PARKER L.C., TANAKA M.
	Mon. Not. R. Astron. Soc., 443, 2679-2694 (2014)
	The GEEC2 spectroscopic survey of Galaxy groups at 0.8 < z < 1.
o	Table 1: <[BMM2014] NNNNNNN> N=9245 among (Nos 26434-1970151).
=E=	Catalogue in electronic form as J/MNRAS/443/2679
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMM2015]
[BMM2015]	(Bellazzini+Magrini+Mucciarelli+, 2015) (Not yet in Simbad)
Write:	<<[BMM2015] SNA>>
N:	4
Note:	LBT MODS1 observations of N=4 nearly point-like sources in a candidate stellar counterpart to the Ultra Compact High Velocity Cloud (UVHVC) HVC 274.68+74.70-123.
Ref:	=2015ApJ...800L..15B
by	BELLAZZINI M. , MAGRINI L., MUCCIARELLI A., BECCARI G., IBATA R., BATTAGLIA G., MARTIN N., TESTA V., FUMANA M., MARCHETTI A., CORRENTI M., FRATERNALI F.
	Astrophys. J., 800L, 15 (2015)
	H II regions within a compact high velocity cloud. A nearly starless dwarf galaxy?
o	Text, Table 2: <SECCO N> (No. 1). Figs 2-3, Table 1: <[BMM2015] SNA> (Nos S2-S3, S3A-S3B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BMP
BMP	(Birkby+Miszalski+Parker)
Write:	<<BMP JHHMM+DDMM>>
N:	78
Object:	PN (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
Stat:	is completely incorporated in Simbad
Note:	Object name consists of the initial letters of the discoverers. See also FPM, MPA.
Ref:	=2008MNRAS.384..525M
by	MISZALSKI B. , PARKER Q.A., ACKER A., BIRKBY J.L., FREW D.J., KOVACEVIC A.
	Mon. Not. R. Astron. Soc., 384, 525-534 (2008)
	MASH-II: more planetary nebulae from the AAO/UKST Hα survey.
o	Table 3: <BMP JHHMM+DDMM> N=78, <FPM JHHMM+DDMM> N=2, <MPA JHHMM+DDMMa> N=255.
=E=	Catalogue in electronic form as V/127
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BMP2002]
[BMP2002]	(Boumis+Mavromatakis+Paleologou+, 2002) (Not yet in Simbad)
Write:	<<[BMP2002] FNa>>
N:	8+4
Object:	Filament (SIMBAD class: PartofCloud = Part of Cloud)
Note:	Filamentary structure in the area of Pegasus constellation.
Ref:	=2002A&A...396..225B
by	BOUMIS P. , MAVROMATAKIS F., PALEOLOGOU E.V., BECKER W.
	Astron. Astrophys., 396, 225-234 (2002)
	New optical filamentary structures in Pegasus.
o	Fig.1, Table 2: <[BMP2002] FNa> (Nos F1-F8, F2a-F2b, F5a-F5b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMP2004]
[BMP2004]	(Bouche+Murphy+Peroux, 2004)
Write:	<<[BMP2004] SDSS JHHMMSS.ss+DDMMSS.s abs N.NNNNN>>
N:	212
Object:	Absorber
Note:	212 MgII absorption systems from SDSS DR1 QSOs selected from HST STIS and GHRS observations in the literature, chosen to overlap with the combined HIPASS catalogue. See also [BMP2006] from SDSS DR3.
Ref:	=2004MNRAS.354L..25B
by	BOUCHE N. , MURPHY M.T., PEROUX C.
	Mon. Not. R. Astron. Soc., 354, 25-29 (2004)
	The clustering of luminous red galaxies around MgII absorbers.
o	Table 1: <[BMP2004] SDSS JHHMMSS.ss+DDMMSS.s abs N.NNNNN> N=212.
=E=	Catalogue in electronic form as J/MNRAS/354/L25
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMP2006]
[BMP2006]	(Bouche+Murphy+Peroux+, 2006) (Not yet in Simbad)
Write:	<<[BMP2006] SDSS JHHMMSS.ss+DDMMSS.s abs N.NNNN>>
N:	1806
Object:	Absorber
Note:	MgII absorption systems from SDSS DR3 SDSS. See also [BMP2004] from SDSS DR1.
Ref:	=2006MNRAS.371..495B
by	BOUCHE N. , MURPHY M.T., PEROUX C., CSABAI I., WILD V.
	Mon. Not. R. Astron. Soc., 371, 495-512 (2006)
	New perspectives on strong z ≃ 0.5 MgII absorbers: are halo mass and equivalent width anticorrelated?
o	Table 1: <[BMP2006] SDSS JHHMMSS.ss+DDMMSS.s abs N.NNNN> N=1806.
=E=	Catalogue in electronic form as J/MNRAS/371/495
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMP2007]
[BMP2007]	(Bouche+Murphy+Peroux+, 2007) (Not yet in Simbad)
Write:	<<[BMP2007] QSO JHHMM+DDMM abs N.NNN>> <<[BMP2007] QSO JHHMM+DDMM abs N.NNNN>> <<[BMP2007] QSO JHHMM+DDMM abs N.NNNNN>>
N:	21
Object:	Absorber
Note:	SINFONI spectrograph observations of MgII absorbers.
Ref:	=2007ApJ...669L...5B
by	BOUCHE N. , MURPHY M.T., PEROUX C., DAVIES R., EISENHAUER F., FORSTER SCHREIBER N.M., TACCONI L.
	Astrophys. J., 669L, 5-8 (2007)
	The SINFONI Mg II program for line emitters (SIMPLE): discovering starbursts near QSO sight lines.
o	Table 1: <[BMP2007] QSO JHHMM+DDMM abs N.NNN>, <[BMP2007] QSO JHHMM+DDMM abs N.NNNN>, <[BMP2007] QSO JHHMM+DDMM abs N.NNNNN>, N=21.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMP2009]
[BMP2009]	(Barrado+Morales-Calderon+Palau+, 2009)= (SSTB213)
Write:	<<[BMP2009] SSTB213 J041757.75+274105.5>> <<[BMP2009] SSTB213 J041757.75+274105.5 A>> <<[BMP2009] SSTB213 J041757>> (not recognised by Simbad, but found in literature) <<[BMP2009] SSTB213 J041757 A>>
N:	1+3
Object:	Poss. Brown Dwarf + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC, Calar Alto OMEGA2000 and VLT ISAAC observations of a proto brown dwarf in the Barnard 213 cloud, in Taurus. See also SSTB213.
in source:	NAME Taurus Region
in source:	Barnard 213
Ref:	=2009A&A...508..859B
by	BARRADO D. , MORALES-CALDERON M., PALAU A., BAYO A., DE GREGORIO-MONSALVO I., EIROA C., HUELAMO N., BOUY H., MORATA O., SCHMIDTOBREICK L.
	Astron. Astrophys., 508, 859-867 (2009)
	A proto brown dwarf candidate in Taurus.
o	<[BMP2009] SSTB213 J041757.75+274105.5> (N=1). <[BMP2009] SSTB213 J041757.75+274105.5 A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMP2010]
[BMP2010]	(Balestra+Mainieri+Popesso+, 2010)
Write:	<<[BMP2010] NNNN>>
N:	4602
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT VIMOS spectroscopy in the GOODS South field. The numbering NNNN (Nos 1-4602), not present in the published catalog, represents the running number of the cleaned catalog ('recno' number in the catalog J/A+A/451/1159).
in source:	NAME GOODS South Field
Ref:	=2010A&A...512A..12B
by	BALESTRA I. , MAINIERI V., POPESSO P., DICKINSON M., NONINO M., ROSATI P., TEIMOORINIA H., VANZELLA E., CRISTIANI S., CESARSKY C., FOSBURY R.A.E., KUNTSCHNER H., RETTURA A.
	Astron. Astrophys., 512A, 12-12 (2010)
	The Great Observatories Origins Deep Survey. VLT/VIMOS spectroscopy in the GOODS-South field: part II.
o	lrv2c.dat,mrv2c.dat: <[BMP2010] NNNN> (Nos 1-4602).
=E=	Catalogue in electronic form as J/A+A/512/A12
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMP2022]
[BMP2022]	(Boyett+Mascia+Pentericci+, 2022) (Not yet in Simbad)
Write:	<<[BMP2022] NNNN>>
N:	15
Object:	Em. G (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	JWST NIRISS/WFSS observations of N=15 emission-line galaxies in the field of Abell 2744, as part of the GLASS-JWST Early Release Science Program.
in source:	ACCG 118 = ACO 2744
Ref:	=2022ApJ...940L..52B
by	BOYETT K. , MASCIA S., PENTERICCI L., LEETHOCHAWALIT N., TRENTI M., BRAMMER G., ROBERTS-BORSANI G., STRAIT V., TREU T., BRADAC M., GLAZEBROOK K., ACEBRON A., BERGAMINI P., CALABRO A., CASTELLANO M., FONTANA A., GRILLO C., HENRY A., JONES T., MARCHESINI D., MASON C., MERCURIO A., MORISHITA T., NANAYAKKARA T., ROSATI P., SCARLATA C., VANZELLA E., VULCANI B., WANG X., WILLOTT C.
	Astrophys. J., 940L, 52 (2022)
	Early Results from GLASS-JWST. VI. Extreme Rest-optical Equivalent Widths Detected in NIRISS Wide Field Slitless Spectroscopy.
o	Table 1: <[BMP2022] NNNN> N=15 among (Nos 320-2707).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMP98]
[BMP98]	(Barret+Motch+Predehl, 1998)
Write:	<<[BMP98] A>>
N:	13
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations. Table 1: N=13 objects in the error box of the burster KS 1731-260 Map in Fig.4
Ref:	=1998A&A...329..965B
by	BARRET D. , MOTCH C., PREDEHL P.
	Astron. Astrophys., 329, 965-970 (1998)
	ROSAT and follow-up infrared observations of the X-ray burster KS 1731-260.
o	p.968: stars 1 and 2 = [CGK94] KS 1731-260 Star 1 and 2
o	Table 1: <[BMP98] A> (Nos A-M).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMR2000]
[BMR2000]	(Blair+Morse+Raymond+, 2000)
Write:	<<[BMR2000] JHHMMSS.s+DDMMSS>>
N:	3
Object:	PairG + G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 and FOS observations of the SMC. 3 background galaxies are observed: the first includes two early-type galaxies, and others are two face-on spirals.
Ref:	=2000ApJ...537..667B
by	BLAIR W.P. , MORSE J.A., RAYMOND J.C., KIRSHNER R.P., HUGHES J.P., DOPITA M.A., SUTHERLAND R.S., LONG K.S., WINKLER P.F.
	Astrophys. J., 537, 667-689 (2000)
	Hubble space telescope observations of oxygen-rich supernova remnants in the Magellanic clouds. II. Elemental abundances in N132D and 1E 0102.2-7219.
o	Text p.670: <[BMR2000] JHHMMSS.s+DDMMSS> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMR2007]
[BMR2007]	(Balog+Muzerolle Rieke+, 2007)
Write:	<<[BMR2007] JDDD.dddd+DD.dddd>>
N:	1084
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Spitzer IRAC observations of NGC 2244.
in source:	NGC 2244
Ref:	=2007ApJ...660.1532B
by	BALOG Z. , MUZEROLLE J., RIEKE G.H., SU K.Y.L., YOUNG E.T., MEGEATH S.T.
	Astrophys. J., 660, 1532-1540 (2007)
	Spitzer/IRAC-MIPS survey of NGC 2244: protostellar disk survival in the vicinity of hot stars.
o	Table 1: <[BMR2007] JDDD.dddd+DD.dddd> N=1084.
=E=	Catalogue in electronic form as J/ApJ/660/1532
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMR2009]
[BMR2009]	(Binder+Markowitz+Rothschild, 2009)
Write:	<<[BMR2009] NN>>
N:	22
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observation of the field of NGC 3226 and NGC 3227.
in source:	NGC 3226
Ref:	=2009ApJ...691..431B
by	BINDER B. , MARKOWITZ A., ROTHSCHILD R.E.
	Astrophys. J., 691, 431-440 (2009)
	A new XMM-Newton long look of the low-luminosity active galactic nucleus NGC 3226.
o	Table 2: <[BMR2009] NN> (Nos 1-22).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMR2018]
[BMR2018]	(Baez-Rubio+Martin-Pintado+Rico-Villas+, 2018)
Write:	<<[BMR2018] 10NE>>
N:	1
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	N=1 ionized source near [LBO2018] 10 in NGC 253, using ALMA archival data at 231.90GHz and 353.62GHz.
in source:	NGC 253
Ref:	=2018ApJ...867L...6B
by	BAEZ-RUBIO A. , MARTIN-PINTADO J., RICO-VILLAS F., JIMENEZ-SERRA I.
	Astrophys. J., 867L, 6-6 (2018)
	Evidence for the first extragalactic hydrogen recombination line maser in NGC 253.
o	Fig. 1, Table 1: <[BMR2018] 10NE> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMS2000]
[BMS2000]	(Bocchino+Maggio+Sciortino+, 2000) (Not yet in Simbad)
Write:	<<[BMS2000] Fil A>>
N:	4
Object:	Filament (SIMBAD class: Region = Region defined in the Sky)
in source:	NAME Vela SNR
Ref:	=2000A&A...359..316B
by	BOCCHINO F. , MAGGIO A., SCIORTINO S., RAYMOND J.
	Astron. Astrophys., 359, 316-336 (2000)
	Multi-wavelength observations and modelling of shock-cloud interaction regions in the Vela Supernova Remnant.
o	Figs, Table 1: <[BMS2000] Fil A> (Nos B-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMS2001]
[BMS2001]	(Bruhweiler+Miskey+Smith+, 2001)= ([BMS2001a]) (Not yet in Simbad)
Write:	<<[BMS2001] Cloud N>>
N:	3
Object:	Cloud (SIMBAD class: Cloud)
Note:	N=3 circumnuclear cloud in NGC 1068.
in source:	NGC 1068
Ref:	=2001ApJ...546..866B
by	BRUHWEILER F.C. , MISKEY C.L., SMITH A.M., LANDSMAN W., MALUMUTH E.
	Astrophys. J., 546, 866-876 (2001)
	Ionization, extinction, and spiral structure in the inner disk of NGC 1068.
o	Table 2, Fig.2: <[BMS2001] Cloud N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMS2001a]
[BMS2001a]	(Bruhweiler+Miskey+Smith+, 2001) (Not yet in Simbad)
*****	Avoid the usage of [BMS2001a], prefer [BMS2001]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMS2001b]
[BMS2001b]	(Budding+Marsden+Slee, 2001)
Write:	<<[BMS2001b] N>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=3 radio-sources in the field of KZ Pav.
Ref:	=2001PASA...18..140B
by	BUDDING E. , MARSDEN S.C., SLEE O.B.
	Publications - Astron. Soc. Australia, 18, 140-147 (2001)
	The active Algol binary KZ Pavonis.
o	Table 2: <[BMS2001b] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMS2003]
[BMS2003]	(Bruhweiler+Miskey+Smith Neubig, 2003)
Write:	<<[BMS2003] yyy>> <<[BMS2003] yyyA>> <<[BMS2003] yyy N>>
N:	49
Object:	* (SIMBAD class: Star)
Note:	HST (STIS, WFPC1, WFPC2) observations of the HII region NGC 604. In the different formats, yyy represent the vertical y-position of the source (in pixels) in the spectral image. The alphabetical extension indicates that there is more than one source near that y-position. The numerical extension indicates two stars located horizontally next to each other.
in source:	NGC 604
Ref:	=2003AJ....125.3082B
by	BRUHWEILER F.C. , MISKEY C.L., SMITH NEUBIG M.
	Astron. J., 125, 3082-3096 (2003)
	STIS spectral imagery of the OB stars in NGC 604. II. The most luminous stars.
o	Fig. 1, Table 2: <[BMS2003] yyy>, <[BMS2003] yyyA>, <[BMS2003] yyy N>, N=49 among (Nos 24-951).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMS2004]
[BMS2004]	(Benetti+Meikkle+Stehle+, 2004) (Not yet in Simbad)
Write:	<<[BMS2004] N>>
N:	6
Object:	* (SIMBAD class: Star)
Note:	N=6 stars in the field of SN 2002BO.
Ref:	=2004MNRAS.348..261B
by	BENETTI S. , MEIKLE P., STEHLE M., ALTAVILLA G., DESIDERA S., FOLATELLI G., GOOBAR A., MATTILA S., MENDEZ J., NAVASARDYAN H., PASTORELLO A., PATAT F., RIELLO M., RUIZ-LAPUENTE P., TSVETKOV D., TURATTO M., MAZZALI P., HILLEBRANDT W.
	Mon. Not. R. Astron. Soc., 348, 261-278 (2004)
	Supernova 2002bo: inadequacy of the single parameter description.
o	Fig.1, Table 1: <[BMS2004] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMS2006]
[BMS2006]	(Bolton+Moustakas+Stern+, 2006)
Write:	<<[BMS2006] J1011+0143 A>> <<[BMS2006] J1011+0143 source>>
N:	4+1+1
Object:	Grav. lensed image + G (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Stat:	is completely incorporated in Simbad
Note:	Keck LRIS observations of SDSS J101129.49+014323.3. Confirmation of a new Einstein cross.
Ref:	=2006ApJ...646L..45B
by	BOLTON A.S. , MOUSTAKAS L.A., STERN D., BURLES S., DEY A., SPINRAD H.
	Astrophys. J., 646, 45-48 (2006)
	A new EINSTEIN cross: a highly magnified, intrinsically faint Lyα emitter at z=2.7.
o	Fig.2, Tables: <[BMS2006] J1011+0143 A> (Nos A-D, G), <[BMS2006] J1011+0143 source> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMS2012]
[BMS2012]	(Brandl+Martin-Hernandez+Schaerer+, 2012)
Write:	<<[BMS2012] MN>>
N:	9 (SIMBAD class: StarFormingReg = Star Forming Region)
Stat:	is completely incorporated in Simbad
Note:	VLT VISIR MIR observations of the starburst ring of NGC 7552.
in source:	NGC 7552
Ref:	=2012A&A...543A..61B
by	BRANDL B.R. , MARTIN-HERNANDEZ N.L., SCHAERER D., ROSENBERG M., VAN DER WERF P.P.
	Astron. Astrophys., 543A, 61-61 (2012)
	High resolution IR observations of the starburst ring in NGC 7552. One ring to rule them all ?
o	Table 2 : <[BMS2012] MN> (Nos 1-9)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMS2015]
[BMS2015]	(Bellazzini+Mucciarelli+Sollima+, 2015)
Write:	<<[BMS2015] NNNN>>
N:	165
Object:	RGB* (SIMBAD class: Star)
Note:	VLT FLAMES spectroscopy of N=165 red giant branch stars in the globular cluster NGC 5694.
in source:	NGC 5694
Ref:	=2015MNRAS.446.3130B
by	BELLAZZINI M. , MUCCIARELLI A., SOLLIMA A., CATELAN M., DALESSANDRO E., CORRENTI M., D'ORAZI V., CORTES C., AMIGO P.
	Mon. Not. R. Astron. Soc., 446, 3130-3138 (2015)
	Kinematics of a globular cluster with an extended profile: NGC 5694.
o	Table 1: <[BMS2015] NNNN> N=165 among (Nos 65 to 1906).
=E=	Catalogue in electronic form as <J/MNRAS/446/3130/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMS2020]
[BMS2020]	(Borsato+Martell+Simpson, 2020) (Not yet in Simbad)
Write:	<<[BMS2020] BGS-N>>
N:	5
Object:	Stellar Stream (SIMBAD class: Stream = Stellar Stream)
Note:	N=5 stellar streams in Gaia DR2 data.
Ref:	=2020MNRAS.492.1370B
by	BORSATO N.W. , MARTELL S.L., SIMPSON J.D.
	Mon. Not. R. Astron. Soc., 492, 1370-1384 (2020)
	Identifying stellar streams in Gaia DR2 with data mining techniques.
o	<[BMS2020] BGS-N> (Nos BGS-1 to BGS-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMS97]
[BMS97]	(Benitez+Martinez-Gonzalez+Sanz+, 1997) (Not yet in Simbad)
Write:	<<[BMS97] NN>>
N:	5
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Non-stellar objects in the field of QSO 0836+113
Ref:	=1997A&A...321..129B
by	BENITEZ N. , MARTINEZ-GONZALEZ E., SANZ J.L., AGUIRRE A., ALISES M.
	Astron. Astrophys., 321, 129-133 (1997)
	The absorbers towards Q0836+113.
o	Table 1, Fig 1: <WTL92] S> N=1. <[BMS97] NN> N=5 among (Nos 6-22)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMS99]
[BMS99]	(Batuski+Miller+Slinglend+, 1999)
Write:	<<[BMS99] JHHMMSS.ss+DDMMSS.s>> <<[BMS99] NNN>>
N:	737
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Tables 1, 2, 3: N=737 galaxies in 31 clusters, format 'JHHMMSS.ss+DDMMSS.s'. Table 4: N=117 galaxies among the 737 are emission-line galaxies, format 'NNN' N=117 among (Nos 1-122).
Ref:	=1999ApJ...520..491B
by	BATUSKI D.J. , MILLER C.J., SLINGLEND K.A., BALKOWSKI C., MAUROGORDATO S., CAYATTE V., FELENBOK P., OLOWIN R.
	Astrophys. J., 520, 491-506 (1999)
	Discovery of extreme examples of superclustering in Aquarius.
o	Tables 1, 2, 3: <[BMS99] JHHMMSS.ss+DDMMSS.s> N=737. Table 4: <[BMS99] NNN> N=117 among (Nos 1-122).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMT2019]
[BMT2019]	(Brownson+Maiolino +Tazzari+, 2019)
Write:	<<[BMT2019] A>>
N:	5
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	N=5 continuum sources in the field of the quasar HE0515-4414. Use of ALMA band 4 archival observations.
Ref:	=2019MNRAS.490.5134B
by	BROWNSON S. , MAIOLINO R., TAZZARI M., CARNIANI S., HENDEN N.
	Mon. Not. R. Astron. Soc., 490, 5134-5146 (2019)
	Detecting the halo heating from AGN feedback with ALMA.
o	Fig. 1, Table 1: <[BMT2019] A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMV2009]
[BMV2009]	(Boyer+McDonald+van Loon+, 2009)
Write:	<<[BMV2009] sNN>>
N:	12
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC and MIPS observations of NGC 362, as part of the SAGE-SMC Spitzer Legacy program.
in source:	NGC 362
Ref:	=2009ApJ...705..746B
by	BOYER M.L. , McDONALD I., VAN LOON J.Th., GORDON K.D., BABLER B., BLOCK M., BRACKER S., ENGELBRACHT C., HORA J., INDEBETOUW R., MEADE M., MEIXNER M., MISSELT K., OLIVEIRA J.M., SEWILO M., SHIAO B., WHITNEY B.
	Astrophys. J., 705, 746-757 (2009)
	Dust production and mass loss in the galactic globular cluster NGC 362.
o	Table 2, Text: <[BMV2009] sNN> (Nos s01-s12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMV2011]
[BMV2011]	(Bayliss+McMahon+Venemans+, 2011)
Write:	<<[BMV2011] DDD.ddddd+DD.ddddd>>
N:	26
Object:	[OII] emitter (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	ESO VLT HAWK-I observations of N=26 [OII] emission line objects in the GOODS South field.
in source:	NAME GOODS South Field
Ref:	=2011MNRAS.413.2883B
by	BAYLISS K.D. , McMAHON R.G., VENEMANS B.P., RYAN-WEBER E.V., LEWIS J.R.
	Mon. Not. R. Astron. Soc., 413, 2883-2894 (2011)
	[O II] emitters in the GOODS field at z~ 1.85: a homogeneous measure of evolving star formation.
o	Table 4: <[BMV2011] DDD.ddddd+DD.ddddd> N=26.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BMW-HRI
BMW-HRI	(Brera Multi-scale Wavelet HRI survey)
Write:	<<BMW-HRI JHHMMSS.s+DDMMSS>>
N:	9 among 154
Object:	Poss. ClG (SIMBAD class: ClG = Cluster of Galaxies)
Note:	Cluster survey based on ROSAT HRI archive. The clusters are selected on the basis of their X-ray extension, measured by the BMW wavelet detection algorith.
Ref:	=2004A&A...428...21M
by	MORETTI A. , GUZZO L., CAMPANA S., LAZZATI D., PANZERA M.R., TAGLIAFERRI G., ARENA S., BRAGLIA F., DELL'ANTONIO I., LONGHETTI M.
	Astron. Astrophys., 428, 21-37 (2004)
	The Brera Multi-scale Wavelet HRI Cluster Survey. I. Selection of the sample and number counts.
o	Text: <BMW-HRI JHHMMSS.s+DDMMSS> N=9 among 154.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 1BMW
1BMW	(Brera Multiscale Wavelet algorithm)
Write:	<<1BMW JHHMMSS.s+DDMMSS>>
N:	29089
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	'BMW' algorithm is developed to analyse high energy astronomical images.
Ref:	=1999A&A...349L...1I
by	ISRAEL G.L. , PANZERA M.R., CAMPANA S., LAZZATI D., COVINO S., TAGLIAFERRI G.
	Astron. Astrophys., 349, 1-4 (1999)
	The discovery of 321s pulsations in the ROSAT HRI light curves of 1BMW J080622.8+152732 = RX J0806.3+1527.
o	<1BMW JHHMMSS.s+DDMMSS> N=1.
Ref:	=2003A&A...399..351P
by	PANZERA M.R. , CAMPANA S., COVINO S., LAZZATI D., MIGNANI R.P., MORETTI A., TAGLIAFERRI G.
	Astron. Astrophys., 399, 351-364 (2003)
	The Brera Multi-scale Wavelet ROSAT HRI source catalogue.
o	Catalog: <1BMW JHHMMSS.s+DDMMSS> N=29089.
=E=	Catalogue in electronic form as IX/34
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BMW93]
[BMW93]	(Baudry+Menten+Walmsley+, 1993)
Write:	<<[BMW93] HHMMSS.sss+DDMMSS.ss>>
N:	1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=1 new source in the field of W 3(OH). See also [DW81] and [GBW85]
in source:	W 3:W 3(OH) = W 3(OH)
Ref:	=1993A&A...271..552B
by	BAUDRY A. , MENTEN K.M., WALMSLEY C.M., WILSON T.L.
	Astron. Astrophys., 271, 552-563 (1993)
	VLA observations of the 8 GHz rotationally excited OH lines toward W 3(OH).
o	Fig.1: OH -VV.V are not in SIMBAD, Masers 1, 2, 3 = [DW81] H2O Maser 1, 2, 3. T.2: Main, Jet and Diffuse = [GBW85] objects.
o	Table 2: <[BMW93] HHMMSS.sss+DDMMSS.ss> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BMZ2001]
[BMZ2001]	(Bejar+Martin+Zapatero Osorio+, 2001)= (S Ori)
Write:	<<[BMZ2001] S Ori JHHMMSS.s+DDMMSS>>
N:	78+1+1+1+48+18+4+19+2+7+23
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Member candidates of the sig Ori cluster. See also [BZR99].
in source:	NAME sig Ori Cluster
Ref:	=2000Sci...290..103Z
by	ZAPATERO OSORIO M.R. , BEJAR V.J.S., MARTIN E.L., REBOLO R., BARRADO Y NAVASCUES D., BAILER-JONES C.A.L., MUNDT R.
	Science, 290, 103-107 (2000)
	Discovery of young, isolated planetary mass objects in the σ Orionis star cluster.
o	Table 1, col(1): <[BZR99] S Ori NN> (Nos 50-69, 59 and 63 missing). Table 1, col(2): <[BMZ2001] S Ori JHHMMSS.s+DDMMSS> N=19 added.
Ref:	=2001ApJ...556..830B
by	BEJAR V.J.S. , MARTIN E.L., ZAPATERO OSORIO M.R., REBOLO R., BARRADO Y NAVASCUES D., BAILER-JONES C.A.L., MUNDT R., BARAFFE I., CHABRIER G., ALLARD F.
	Astrophys. J., 556, 830-836 (2001)
	The substellar mass function in σ Orionis.
o	CHABRIER C. misprint for CHABRIER G.
o	Table 1: <[BMZ2001] S Ori JHHMMSS.s+DDMMSS> N=78
Ref:	=2002ApJ...578..536Z
by	ZAPATERO OSORIO M.R. , BEJAR V.J.S., MARTIN E.L., REBOLO R., BARRADO Y NAVASCUES D., MUNDT R., EISLOEFFEL J., CABALLERO J.A.
	Astrophys. J., 578, 536-542 (2002)
	A methane, isolated, planetary-mass object in Orion.
o	<[BZR99] S Ori NN> (No. 70) added. <[BMZ2001] S Ori JHHMMSS.s+DDMMSS> N=1 added.
Ref:	=2002A&A...393L..85B
by	BARRADO Y NAVASCUES D. , ZAPATERO OSORIO M.R., MARTIN E.L., BEJAR V.J.S., REBOLO R., MUNDT R.
	Astron. Astrophys., 393, 85-88 (2002)
	Discovery of a very cool object with extraordinarily strong Hα emission.
o	PC 0025+0047 is a misprint for PC 0025+0447.
o	<[BZR99] S Ori NN> (No. 71) added. <[BMZ2001] S Ori JHHMMSS.s+DDMMSS> N=1 added.
Ref:	=2003A&A...404..171B
by	BARRADO Y NAVASCUES D. , BEJAR V.J.S., MUNDT R., MARTIN E.L., REBOLO R., ZAPATERO OSORIO M.R., BAILER-JONES C.A.L.
	Astron. Astrophys., 404, 171-185 (2003)
	The σ Orionis substellar population. VLT/FORS spectroscopy and 2MASS photometry.
o	Table 1: <[BMZ2001] S Ori JHHMMSS.s+DDMMSS> N=1 added.
Ref:	=2004AN....325..705B
by	BEJAR V.J.S. , ZAPATERO OSORIO M.R., REBOLO R.
	Astron. Nachr., 325, 705-713 (2004)
	Optical and infrared photometry of new very low-mass stars and brown dwarfs in the σ Orionis cluster.
o	Table 2: <[BMZ2001] S Ori JHHMMSS.s+DDMMSS> N=48 added.
Ref:	=2006A&A...460..799G
by	GONZALEZ-GARCIA B.M. , ZAPATERO OSORIO M.R., BEJAR V.J.S., BIHAIN G., BARRADO Y NAVASCUES D., CABALLERO J.A., MORALES-CALDERON M.
	Astron. Astrophys., 460, 799-810 (2006)
	A search for substellar members in the Praesepe and σ Orionis clusters.
o	Table 5: <[GZB2006] Prae JHHMMSS.s+DDMMSS> N=20. Table 6: <[BMZ2001] S Ori JHHMMSS.s+DDMMSS> N=18 added.
Ref:	=2007A&A...470..903C
by	CABALLERO J.A. , BEJAR V.J.S., REBOLO R., EISLOEFFEL J., ZAPATERO OSORIO M.R., MUNDT R., BARRADO Y NAVASCUES D., BIHAIN G., BAILER-JONES C.A.L., FORVEILLE T., MARTIN E.L.
	Astron. Astrophys., 470, 903-918 (2007)
	The substellar mass function in σ Orionis. II. Optical, near-infrared and IRAC/Spitzer photometry of young cluster brown dwarfs and planetary-mass objects.
o	Table 3: <[BMZ2001] S Ori JHHMMSS.s+DDMMSS> N=4 added.
Ref:	=2009A&A...506.1169B
by	BIHAIN G. , REBOLO R., ZAPATERO OSORIO M.R., BEJAR V.J.S., VILLO-PEREZ I., DIAZ-SANCHEZ A., PEREZ-GARRIDO A., CABALLERO J.A., BAILER-JONES C.A.L., BARRADO Y NAVASCUES D., EISLOEFFEL J., FORVEILLE T., GOLDMAN B., HENNING T., MARTIN E.L., MUNDT R.
	Astron. Astrophys., 506, 1169-1182 (2009)
	Candidate free-floating super-Jupiters in the young σ Orionis open cluster.
o	Table 4: <[BZR99] S Ori NN> (Nos 72-74) added. Table 5: <[BMZ2001] S Ori JHHMMSS.s+DDMMSS> N=2 added.
Ref:	=2011A&A...532A..42P
by	PENA RAMIREZ K. , ZAPATERO OSORIO M.R., BEJAR V.J.S., REBOLO R., BIHAIN G.
	Astron. Astrophys., 532A, 42-42 (2011)
	Search and characterization of T-type planetary mass candidates in the σ Orionis cluster.
o	Tables 4-5: <[BMZ2001] S Ori JHHMMSS.s+DDMMSS> N=1+6.
Ref:	=2012ApJ...754...30P
by	PENA RAMIREZ K. , BEJAR V.J.S., ZAPATERO OSORIO M.R., PETR-GOTZENS M.G., MARTIN E.L.
	Astrophys. J., 754, 30 (2012)
	New isolated planetary-mass objects and the stellar and substellar mass function of the σ Orionis cluster.
o	Table 8: <[BMZ2001] S Ori JHHMMSS.s+DDMMSS> N=20. Tables 4+9+11: <[PBZ2012] JHHMMSS.ss+DDMMSS.s> N=30+14+4.
=E=	Catalogue in electronic form as J/other/AN/325.705
=E=	Catalogue in electronic form as <J/ApJ/754/30/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BN
BN	(Becklin+Neugebauer)
*****	Avoid the usage of BN, prefer BNKL
Details on Acronym: BN
BN	(Becklin+Neugebauer)
*****	Avoid the usage of BN, prefer GCIRS
Origin	of the Acronym: L (1984MNRAS.208..661B)
Details on Acronym: [BN2010]
[BN2010]	(Bloom+Nugent, 2010)
Write:	<<[BN2010] J101648.52-123357.5>>
N:	1 (SIMBAD class: Galaxy)
Note:	Palomar Observatory imaging from the DeepSky* project. Host galaxy of GRB 100219A.
Ref:	=2010GCN.10433....1B
by	BLOOM J.S. , NUGENT P.E.
	GCN, 0433, 1 (2010)
	GRB 100219A: pre-explosion imaging and host candidate.
o	<[BN2010] J101648.52-123357.5> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BNA2015]
[BNA2015]	(Brown+Neff+Ayres+, 2015)
Write:	<<[BNA2015] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	Dwarf Nova (SIMBAD class: CataclyV* = Cataclysmic Binary)
Note:	Kepler Guest Observer observations of N=1 dwarf nova near the G dwarf KIC 5438845.
Ref:	=2015AJ....149...67B
by	BROWN A. , NEFF J.E., AYRES T.R., KOWALSKI A., HAWLEY S., BERDYUGINA S., HARPER G.M., KORHONEN H., PISKUNOV N., SAAR S., WALKOWICZ L., WELLS M.A.
	Astron. J., 149, 67 (2015)
	Serendipitous discovery of a dwarf nova in the Kepler field near the G dwarf KIC 5438845.
o	<[BNA2015] J191511.79+403626.4> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BNB2006]
[BNB2006]	(Blondin+Narayan+Bloom+, 2006)
Write:	<<[BNB2006] object A>>
N:	3
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Magellan Clay 6.5m telescope LDSS3 spectroscopic observations of the cluster ACO S 995. See also [B2007c].
in source:	ACO S 995
Ref:	=2006GCN..5944....1B
by	BLONDIN S. , NARAYAN G., BLOOM J.S., CHEN H.-.W., KIRSHNER R.P., CHALLIS P., HICKEN M., MODJAZ M., FRIEDMAN A., WOOD-VASEY M., PROCHASKA J.X.
	GCN, 5944, 1 (2006)
	GRB 061201: magellan redshift of nearby Abell cluster.
o	ACO 995 is a misprint for ACO S 995. Coordinates of [BNB2006] object A are corrected in 2006GCN..5945....1B.
o	<[BNB2006] object A> (Nos A, B, D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BNC2010]
[BNC2010]	(Billot+Noriega-Crespo+Carey+, 2010)
Write:	<<[BNC2010] VulPNN>>
N:	14
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=14 pillar-like structures in the Vulpecula OB association. Use of Spitzer MIPSGAL and GLIMPSE data.
in source:	NAME ASS VUL OB 1-
Ref:	=2010ApJ...712..797B
by	BILLOT N. , NORIEGA-CRESPO A., CAREY S., GUIEU S., SHENOY S., PALADINI R., LATTER W.
	Astrophys. J., 712, 797-812 (2010)
	Young stellar objects and triggered star formation in the Vulpecula OB association.
o	Tables 3-4: <[BNC2010] VulPNN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BNE2014]
[BNE2014]	(Belli+Newman+Ellis, 2014)
Write:	<<[BNE2014] DDD.ddddd+DD.dddd>>
N:	56
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck I LRIS spectroscopy of N=56 quiescent galaxies with 0.9<z<1.6. Use of data from the NEWFIRM Medium-Band Survey (NMBS), the MUSYC survey, the WIRCam Deep Survey (WIRDS). Use of Spitzer and Chandra archives.
Ref:	=2014ApJ...783..117B
by	BELLI S. , NEWMAN A.B., ELLIS R.S.
	Astrophys. J., 783, 117 (2014)
	Velocity dispersions and dynamical masses for a large sample of quiescent galaxies at z > 1: improved measures of the growth in mass and size.
o	Table 2: <[BNE2014] DDD.ddddd+DD.dddd> N=56.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BNJ2003]
[BNJ2003]	(Burningham+Naylor+Jeffries+, 2003)
Write:	<<[BNJ2003] XMM NNN>> <<[BNJ2003] XMM NNNa>> <<[BNJ2003] ROSAT NN>>
N:	110+28+13
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Photometric catalog towards the open cluster Cl Collinder 121. Stars in table 1 are 'Cl* Collinder 121 BNJ N-NNNN' in SIMBAD. XMM and ROSAT sources are cross-identified.
Ref:	=2003MNRAS.346.1143B
by	BURNINGHAM B. , NAYLOR T., JEFFRIES R.D., DEVEY C.R.
	Mon. Not. R. Astron. Soc., 346, 1143-1150 (2003)
	On the nature of Collinder 121: insights from the low-mass pre-main sequence.
o	Table 1: <Cl* Collinder 121 BNJ N-NNNN> N=27502. Table 2: <[BNJ2003] XMM NNN> N=110 among (Nos 1-152), <[BNJ2003] XMM NNNs> N=28 among (Nos 4s-118s). Table 3: <[BNJ2003] ROSAT NN> N=13 among (Nos 1-39).
=E=	Catalogue in electronic form as J/MNRAS/346/1143
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BNKL
BNKL	(Becklin+Neugebauer+Kleinmann+Low)= (BN) = (KL)
Write:	<<BNKL N>>
N:	1
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	N=1 extended source, lambda = 22mu.m. The KL source contains the BN object of ref. 1967ApJ...147..799B both are named BNKL in the literature.
in source:	NAME Orion Nebula
Ref:	=1967ApJ...147..799B
by	BECKLIN E.E. , NEUGEBAUER G.
	Astrophys. J., 147, 799-802 (1967)
	Observations of an infrared star in the Orion nebula.
o	<BNKL 1>
Ref:	=1967ApJ...149L...1K
by	KLEINMANN D.E. , LOW F.J.
	Astrophys. J., 149, 1-4 (1967)
	Discovery of an infrared nebula in Orion.
o	<BNKL 1>
Details on Acronym: [BNL2005]
[BNL2005]	(Burningham+Naylor+Littlefair+, 2005)
*****	Avoid the usage of [BNL2005], prefer [KJN2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BNM2012]
[BNM2012]	(Bell+Naylor+Mayne+, 2012)
Write:	<<[BNM2012] FF.FF NNNNN>>
N:	55132+12142+179
Object:	* (SIMBAD class: Star)
Note:	INT WFC observations of N=55132 stars in the Pleiades and N=12142 main-sequence stars in the SDSS Stripe 82.
Ref:	=2012MNRAS.424.3178B
by	BELL C.P.M. , NAYLOR T., MAYNE N.J., JEFFRIES R.D., LITTLEFAIR S.P.
	Mon. Not. R. Astron. Soc., 424, 3178-3191 (2012)
	Pre-main-sequence isochrones. I. The Pleiades benchmark.
o	Tables 2+4+5: <[BNM2012] FF.FF NNNNN> N=55132+12142+179.
=E=	Catalogue in electronic form as J/MNRAS/424/3178
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BNM2013]
[BNM2013]	(Bell+Naylor+Mayne+, 2013)
Write:	<<[BNM2013] FF.FF NNNNN>>
N:	666772
Object:	* (SIMBAD class: Star)
Note:	INT 2.5m telescope observations of N=666772 stars in thirteen young star-forming regions. For more information, visit http://www.astro.ex.ac.uk/people/timn/Catalogues/
in source:	M 16 = Eagle Nebula = NGC 6611
in source:	IC 5146
in source:	NGC 6530 = M 8 = Lagoon Nebula
in source:	NGC 2244
in source:	NAME sig Ori Association
in source:	NAME Ass Cep OB 3b
in source:	IC 348
in source:	NAME lam Ori Cloud
in source:	NGC 2169
in source:	NGC 2362
in source:	NGC 7160
in source:	chi Per Cluster = NGC 884
in source:	NGC 1960 = M 36
Ref:	=2013MNRAS.434..806B
by	BELL C.P.M. , NAYLOR T., MAYNE N.J., JEFFRIES R.D., LITTLEFAIR S.P.
	Mon. Not. R. Astron. Soc., 434, 806-831 (2013)
	Pre-main-sequence isochrones - II. Revising star and planet formation time-scales.
o	Tables 9-34: <[BNM2013] FF.ff NNNNN> N=666772.
=E=	Catalogue in electronic form as J/MNRAS/434/806
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BNM92]
[BNM92]	(Bronkalla+Notni+Mutter, 1992)
Write:	<<[BNM92] BKNN>> <<[BNM92] HN>> <<[BNM92] ExNN>>
N:	39+6+18
Object:	Knot + HII + Hole (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Photographic UBV photometry of NGC 2976. N=39 Bright Knots (format BKNN). N=6 HII regions (format HN). N=18 faint extinction regions or holes (format ExNN).
in source:	NGC 2976
Ref:	=1992AN....313....1B
by	BRONKALLA W. , NOTNI P., MUTTER A.A.-R.
	Astron. Nachr., 313, 1-None (1992)
	Stellar populations and dust in the galaxy NGC 2976, a low-luminosity member of the M 81 group.
o	Table 2: <[BNM92] BKNN> (Nos BK1-BK39). Table 3: <[BNM92] HN> (Nos H1-H6). Table 4: <[BNM92] ExNN> (Nos Ex1-Ex18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BNM96]
[BNM96]	(Bronfman+Nyman+May, 1996)
Write:	<<[BNM96] LLL.lll+B.bbb>>
N:	718
Object:	HII (SIMBAD class: HIIReg = HII Region)
Ref:	=1996A&AS..115...81B
by	BRONFMAN L. , NYMAN L.-A., MAY J.
	Astron. Astrophys., Suppl. Ser., 115, 81-95 (1996)
	A CS(2-1) survey of IRAS point sources with color characteristics of ultra-compact HII regions.
o	misprints IRAS 06361-0147 for 06361-0142, 08533-4418 for 08533-4417, 17180-3316 for 17280-3316.
o	Table 1: <[BNM96] LLL.lll+B.bbb> N=1449
=E=	Catalogue in electronic form as J/A+AS/115/81
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BNR2017]
[BNR2017]	(Berghea+Nelson+Rusu+, 2017)
Write:	<<[BNR2017] J014710+463040 system>> <<[BNR2017] J014710+463040 source>> <<[BNR2017] J014710+463040 A>>
N:	1+1+5
Object:	Poss. Grav. lens system + QSO + Poss. Grav. lensed image of a QSO + Poss. Grav. lens (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=1 gravitational lens system candidate with N=4 gravitationally lensed images of a quasar and N=1 gravitational lens candidate. Use of Pan-STARRS PS1 data.
Ref:	=2017ApJ...844...90B
by	BERGHEA C.T. , NELSON G.J., RUSU C.E., KEETON C.R., DUDIK R.P.
	Astrophys. J., 844, 90-90 (2017)
	Discovery of the first quadruple gravitationally lensed quasar candidate with Pan-STARRS.
o	Fig. 1, Table 1: <[BNR2017] J014710+463040 system> N=1, <[BNR2017] J014710+463040 source> N=1, <[BNR2017] J014710+463040 A> (Nos A-D, G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BO
BO	(Butcher+Oemler)
*****	Avoid the usage of BO, prefer [BO85]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BO
BO	(Butcher+Oemler)
*****	Avoid the usage of BO, prefer BOI
Origin	of the Acronym: L (1991A&AS...91....1P)
Details on Acronym: Bo
Bo	(Bologna obs.)
*****	Avoid the usage of Bo, prefer Bol
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Bo
Bo	(Borngen)
*****	Avoid the usage of Bo, prefer Borngen
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BO
BO	(Butcher+Oemler+)
*****	Avoid the usage of BO, prefer BOW
Origin	of the Acronym: L (1987MNRAS.229..423C)
Details on Acronym: Bo
Bo	(Bochum astr. inst.)
*****	Avoid the usage of Bo, prefer Bochum
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BO85]
[BO85]	(Butcher+Oemler, 1985)= (B) = (BO)
Write:	<<[BO85] ACO NNNN NNN>> <<[BO85] Coma NNN>> <<[BO85] Herc NNN>>
N:	1422
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table 2: format 'ACO 262 NN', N=48 Table 3: format 'ACO 400 NN', N=92' Table 4: format 'ACO 401 NNN', N=140' Table 5: format 'ACO 1367 NNN', N=161' Table 6: format 'Coma NNN', N=321' Table 7: format 'ACO 1904 NNN', N=114' Table 8: format 'Herc NNN', N=147' Table 9: format 'ACO 2199 NNN', N=163' Table 10: format 'ACO 2634 NNN', N=109' Table 11: format 'ACO 2670 NNN', N=127' Paper IV, see also paper I: BOI
in source:	ACO 262
in source:	ACO 400
in source:	ACO 401
in source:	ACO 1367
in source:	ACO 1904
in source:	ACO 2199
in source:	ACO 2634
in source:	ACO 2670
in source:	Coma Cluster = ACO 1656
in source:	NAME Hercules Cluster
Ref:	=1985ApJS...57..665B
by	BUTCHER H.R. , OEMLER A.
	Astrophys. J., Suppl. Ser., 57, 665-691 (1985)
	The evolution of galaxies in clusters. IV. Photometry of 10 low-redshift clusters.
o	Table 2: <[BO85] ACO 262 NN> N=48, Table 3: <[BO85] ACO 400 NN> N=92, Table 4: <[BO85] ACO 401 NNN> N=140, Table 5: <[BO85] ACO 1367 NNN> N=161, Table 6: <[BO85] Coma NNN> N=321, Table 7: <[BO85] ACO 1904 NNN> N=114, Table 8: <[BO85] Herc NNN> N =147, Table 9: <[BO85] ACO 2199 NNN> N=163, Table 10: <[BO85] ACO 2634 NNN> N=109, Table 11: <[BO85] ACO 2670 NNN> N=127
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BO98]
[BO98]	(Burkert+O'Dell, 1998)= (CK)
Write:	<<[BO98] Helix SSs-MSS>>
N:	47
Object:	Knot (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations The authors adopt the system of designation proposed in O'Dell+ 1997, IAU Symposium 180, p. 332: 'Helix SSs-MSS' with a format based on 2000 coordinates, '20h 45 SSs -20 4M SS'. See also [OBH2002].
in source:	Helix Nebula = NGC 7293
Ref:	=1998ApJ...503..792B
by	BURKERT A. , O'DELL C.R.
	Astrophys. J., 503, 792-797 (1998)
	The structure of cometary knots in the Helix Nebula.
o	Table 1: <[BO98] Helix SSs-MSS> N=8
Ref:	=2001ApJ...548..288L
by	LOPEZ-MARTIN L. , RAGA A.C., MELLEMA G., HENNEY W.J., CANTO J.
	Astrophys. J., 548, 288-295 (2001)
	Photoevaporating flows from the cometary knots in the Helix Nebula (NGC 7293).
o	Table 1: <[BO98] Helix SSs-MSS> N=20 added.
Ref:	=2002AJ....123.3329O
by	O'DELL C.R. , BALICK B., HAJIAN A.R., HENNEY W.J., BURKERT A.
	Astron. J., 123, 3329-3347 (2002)
	Knots in nearby planetary nebulae.
o	Fig.10: <[BO98] Helix SSs-MSS> N=18 added. Fig.10: <[OBH2002] AN> (Nos M1-M3).
Ref:	=2006ApJ...652..426H
by	HORA J.L. , LATTER W.B., SMITH H.A., MARENGO M.
	Astrophys. J., 652, 426-441 (2006)
	Infrared observations of the Helix planetary nebula.
o	(Erratum) erratum vol. 656, p. 629 (2007)
o	Table 5: numerotation N (Nos 1-4) is not used in SIMBAD.
o	Table 5, col(2): <[BO98] Helix SSs-MSS> N=1 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BOA98]
[BOA98]	(Brosch+Ofek+Almoznino+, 1998)= (FAUST) = (FSC)
Write:	<<[BOA98] NN>>
N:	56
Object:	G + * (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	FAUST observations of N=7 galaxies and N=49 stars in the Coma cluster See also [BFA97]
in source:	Coma Cluster = ACO 1656
Ref:	=1998MNRAS.295..959B
by	BROSCH N. , OFEK E.O., ALMOZNINO E., SASSEEN T., LAMPTON M., BOWYER S.
	Mon. Not. R. Astron. Soc., 295, 959-969 (1998)
	FAUST observations of ultraviolet sources in the direction of Coma.
o	Table 1: <[BOA98] NN> (Nos 1-56)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BOB2000]
[BOB2000]	(Bica+Ortolani+Barbuy, 2000) (Not yet in Simbad)
Write:	<<[BOB2000] NNN>> <<[BOB2000] Red Giant N>>
N:	735+5
Object:	Giant * (SIMBAD class: Star)
Note:	Table 3: B, V photometry of UKS2 for whole frame. Table 4: Red giants.
in source:	NAME UKS 2
Ref:	=2000A&AS..145..399B
by	BICA E. , ORTOLANI S., BARBUY B.
	Astron. Astrophys., Suppl. Ser., 145, 399-403 (2000)
	B and V photometry of the faint open cluster. UKS 2 (BH 66).
o	Table 3: <[BOB2000] NNN> (Nos 1-735). Table 4: <[BOB2000] Red Giant N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BOB2008]
[BOB2008]	(Beelen+Omont+Bavouzet+, 2008)
Write:	<<[BOB2008] LNN>>
N:	32
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	Large APEX Bolometer Camera (LABoCa) on the Atacama Pathfinder EXperiment (APEX) telescope. Search for 870mu.m sources around ClG J2143-4423.
in source:	ClG J2143-4423
Ref:	=2008A&A...485..645B
by	BEELEN A. , OMONT A., BAVOUZET N., KOVACS A., LAGACHE G., DE BREUCK C., WEISS A., MENTEN K.M., COLBERT J.W., DOLE H., SIRINGO G., KREYSA E.
	Astron. Astrophys., 485, 645-655 (2008)
	Submillimeter observations of the J2142-4423 Lyα protocluster at z = 2.38.
o	J2142-4423 (protocluster) is a misprint for J2143-4423 (ClG J2143-4423 in SIMBAD).
o	Table 1, col(1): <LABoCa JHHMMSS+DDMMSS> N=32, = Table 1, col(2): <[BOB2008] LNN> (Nos L01-L32).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BOB97]
[BOB97]	(Bowen+Osmer+Blades+, 1997)
Write:	<<[BOB97] QHHMM+DDMM GNN>>
N:	30
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=30 G close to 9 bright QSO lines of sight. Maps in Figs 1-5 See also [BBP95], [BBP96]
Ref:	=1997MNRAS.284..599B
by	BOWEN D.V. , OSMER S.J., BLADES J.C., TYTLER D.
	Mon. Not. R. Astron. Soc., 284, 599-606 (1997)
	Redshifts of galaxies close to bright QSO lines of sight.
o	Table 1, maps: <[BOB97] QHHMM+DDMM GNN> N=30
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BoBn
BoBn	(Boeshaar+Bond)= (BB)
Write:	<<PN BoBn N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	BoBn 1 = PN G108.4-76.1 = PK 108-76 1
Ref:	=1977ApJ...213..421B
by	BOESHAAR G.O. , BOND H.E.
	Astrophys. J., 213, 421-426 (1977)
	Chemical abundances of a new halo planetary nebulae.
o	<PN BoBn N> (No. 1).
Details on Acronym: [BOC2010]
[BOC2010]	(Bongiovanni+Oteo+Cepa+, 2010)
Write:	<<[BOC2010] ALHNNNNN>>
N:	16
Object:	LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	N=16 LAEs from the ALHAMBRA survey. Use of Herschel PACS data.
Ref:	=2010A&A...519L...4B
by	BONGIOVANNI A. , OTEO I., CEPA J., PEREZ GARCIA A.M., SANCHEZ-PORTAL M., EDEROCLITE A., AGUERRI J.A.L., ALFARO E.J., ALTIERI B., ANDREANI P., APARICIO-VILLEGAS M.T., AUSSEL H., BENITEZ N., BERTA S., BROADHURST T., CABRERA-CANO J., CASTANDER F.J., CAVA A., CERVINO M., CHULANI H., CIMATTI A., CRISTOBAL-HORNILLOS D., DADDI E., DOMINGUEZ H., ELBAZ D., FERNANDEZ-SOTO A., FOERSTER SCHREIBER N., GENZEL R., GOMEZ M.F., GONZALEZ DELGADO R.M., GRAZIAN A., GRUPPIONI C., HERREROS J.M., IGLESIAS GROTH S., INFANTE L., LUTZ D., MAGNELLI B., MAGDIS G., MAIOLINO R., MARQUEZ I., MARTINEZ V.J., MASEGOSA J., MOLES M., MOLINO A., NORDON R., DEL OLMO A., PEREA J., POGLITSCH A., POPESSO P., POZZI F., PRADA F., QUINTANA J.M., RIGUCCINI L., RODIGHIERO G., SAINTONGE A., SANCHEZ S.F., SANTINI P., SHAO L., STURM E., TACCONI L., VALTCHANOV I.
	Astron. Astrophys., 519L, 4-4 (2010)
	Herschel FIR counterparts of selected Lyα emitters at z ~ 2.2. Fast evolution since z ~ 3 or missed obscured AGNs?
o	Fig. B.1, Table B.1: <[BOC2010] ALHNNNNN> N=16 among (Nos 00228-11687).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Bochum
Bochum	(Bochum astr. inst.)= (Bo)
Write:	<<Cl Bochum NN>>
N:	15
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Stat:	is completely incorporated in Simbad
Ref:	=1975A&AS...20...85M
by	MOFFAT A.F.J. , VOGT N.
	Astron. Astrophys., Suppl. Ser., 20, 85-124 (1975)
	Southern open star clusters. IV. UBV Hβ photometry of 26 clusters from Monoceros to Vela.
o	Table 2 in Cl Bochum 1, and Table 13 in Cl Bochum 6: objects 'NNN' are 'LS NNN' in SIMBAD.
o	Table 3: <NGC 2186 NN> N=23. Table 4: <Cl Collinder 96 NN> N=14. Table 5: <NGC 2269 NN> N=12. Table 6: <Cl Biurakan 10 N> N=4. Table 7: <Cl Dolidze 25 NN> N=23. Table 8: <Cl Bochum 2 N> N=8. Table 9: <Cl Bochum 3 N> N=8. Table 10: <NGC 2302 NN> N=16. Table 11: <Cl* Haffner 8 MV NN> N=13. Table 12: <Cl Bochum 4 NN> = <Cl Bochum 5 NN> N=30. Table 14: <NGC 2421 NN> N=28. Table 15: <Cl Ruprecht 34 NN> N=17. Table 16: <Cl Ruprecht 18 NN> N=20. Table 17: <Cl Ruprecht 32 NN> N=16. Table 18: <NGC 2482 NN> N=41. Table 19: <Cl Ruprecht 55 NN> N=18. Table 21: <Cl Pismis 4 NN> N=16. Table 22: <Cl Ruprecht 67 NN> N=27. Table 24: <Cl Pismis 12 NN> N=17. Table 27: <Cl Ruprecht 79 NN> N=22. Table 27: <Cl Bochum N> (Nos 1-7).
Ref:	=1975A&AS...20..125M
by	MOFFAT A.F.J. , VOGT N.
	Astron. Astrophys., Suppl. Ser., 20, 125-153 (1975)
	Southern open star clusters. V. UBV Hβ photometry of 20 clusters in Carina.
o	Tables 1-20: <Cl Bochum 8 N> N=8. <Cl Westerlund 2 N> N=9. <NGC 3255 N> N=8. <Cl* NGC 3324 MV NN> N=12. <Cl Bochum 9 NN> N=22. <Cl Bochum 10 NN> N=17. <Cl Bochum 11 N> N=8. <Cl Hogg 9 N> N=9. <Cl Pismis 17 N> N=9. <Cl Sher 1 NN> N=11. <Cl Bochum 12 NN> N=12. <Cl Stock 13 NN> N=23. <Cl* NGC 3572 MV NN> N=30. <Cl* Hogg 10 MV NN> N=11. <Cl Hogg 11 N> N=6. <Cl* Trumpler 18 MV NN> N=31. <Cl Hogg 12 NN> N=11. <Cl* NGC 3590 MV NN> N=21. <Cl Stock 14 NN> N=21. <Cl Ruprecht 97 NN> N=33. <Cl Bochum NN> (Nos 8-12).
Ref:	=1975A&AS...20..155M
by	MOFFAT A.F.J. , VOGT N.
	Astron. Astrophys., Suppl. Ser., 20, 155-182 (1975)
	Southern open star clusters. VI. UBV Hβ photometry of 18 clusters from Centaurus to Sagittarius.
o	Table 1: <Cl Collinder 268 NN> N=22. Table 2: <Cl Ruprecht 107 NN> N=17. Table 4: <Cl Lynga 4 N> N=6. Table 5: <NGC 6005 N> N=6. Table 7: <Cl Lynga 6 NN> N=18. Table 8: <Cl Collinder 307 NN> N=12. Table 9: <Cl* NGC 6167 MV NN> N=21. Table 10: <NGC 6250 NN> N=28. Table 11: <Cl Lynga 14 NN> N=16. Table 13: <Cl Bochum 13 NN> N=12. Table 14: <Cl Ruprecht 127 NN> N=18. Table 15: <NGC 6396 NN> N=22. Table 16: <Cl Collinder 347 NN> N=20. Table 17: <Cl Bochum 14 NN> N=11. Table 18: <NGC 6604 NN> N=11. Table 20: <Cl Bochum NN> (Nos 13-14).
Ref:	=1976A&A....46..287F
by	FITZGERALD M.P. , HURKENS R., MOFFAT A.F.J.
	Astron. Astrophys., 46, 287-291 (1976)
	Bochum 15, a new young stellar aggregate in Puppis.
o	<Cl Bochum 15>. Table 1: <Cl Bochum 15 NN> (Nos 1-38).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BOD2015]
[BOD2015]	(Baug+Ojha+Dewangan+, 2015)
Write:	<<[BOD2015] A>> <<[BOD2015] JHHMMSS.sss+DDMMSS.sss>>
N:	150+5
Object:	YSO + Clumps (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Himalayan Chandra 2m telescope (HCT, India) NIR-spectrophotometric observations and GMRT 1280MHz radio continuum observations of N=151+5 YSOs and radio clumps in the Sh2-138 region. Use of UKIDSS and WISE archival data.
in source:	SH 2-138
Ref:	=2015MNRAS.454.4335B
by	BAUG T. , OJHA D.K., DEWANGAN L.K., NINAN J.P., BHATT B.C., GHOSH S.K., MALLICK K.K.
	Mon. Not. R. Astron. Soc., 454, 4335-4356 (2015)
	Sh2-138: physical environment around a small cluster of massive stars.
o	Table S1: <[BOD2015] JHHMMSS.sss+DDMMSS.sss> N=151. Table 2: <[BOD2015] A> (Nos A-E).
=E=	Catalogue in electronic form as J/MNRAS/454/4335
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BOD99]
[BOD99]	(Bloom+Odewahn+Djorgovski+, 1999)
Write:	<<[BOD99] Galaxy A>> <<[BOD99] Knot AN>>
N:	1+3
Object:	G + Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST and Keck observations of GRB 990123. N=1 G, the host galaxy of GRB 990123. See alos [OBK99]. N=2 knots associated with the galaxy, Knot A1 and Knot B. N=1 nebulosity, may be a star-forming region: Knot A2. See also [HH99].
Ref:	=1999ApJ...518L...1B
by	BLOOM J.S. , ODEWAHN S.C., DJORGOVSKI S.G., KULKARNI S.R., HARRISON F.A., KORESKO C., NEUGEBAUER G., ARMUS L., FRAIL D.A., GAL R.R., SARI R., SQUIRES G., ILLINGWORTH G., KELSON D., CHAFFEE F.H., GOODRICH R., FEROCI M., COSTA E., PIRO L., FRONTERA F., MAO S., AKERLOF C., McKAY T.A.
	Astrophys. J., 518, 1-4 (1999)
	The host galaxy of GRB 990123.
o	Figs 1, 2: Objects G, L, M are not in SIMBAD.
o	Fig.2: <[BOD99] Galaxy A>, <[BOD99] Knot AN> (Nos A1-A2, B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BOF2008]
[BOF2008]	(Boomsma+Oosterloo+Fraternali+, 2008) (Not yet in Simbad)
Write:	<<[BOF2008] NNN>>
N:	121
Object:	HI Hole (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	WSRT observations of NGC 6946.
in source:	NGC 6946
Ref:	=2008A&A...490..555B
by	BOOMSMA R. , OOSTERLOO T.A., FRATERNALI F., VAN DER HULST J.M., SANCISI R.
	Astron. Astrophys., 490, 555-570 (2008)
	HI holes and high-velocity clouds in the spiral galaxy NGC6946.
o	Fig.7: <[BOF2008] NNN> (Nos 1-121).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BOI
BOI	(Butcher+Oemler, paper I)= (BO)
Write:	<<BOI Cl 0024+1654 NNN>> <<BOI 3C 295 NNN>>
N:	136+107
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Table 1: format 'Cl 0024+1654 NNN', N=136 G in Cl 0024+1654 Table 2: format '3C 295 NNN', N=107 G in NAME 3C 295 Cluster Paper I, see also paper IV: [BO85]
in source:	NAME 3C 295 Cluster
in source:	ClG 0024+1652 = HMS 0024+1654
Ref:	=1978ApJ...219...18B
by	BUTCHER H. , OEMLER A.Jr
	Astrophys. J., 219, 18-30 (1978)
	The evolution of galaxies in clusters. I. ISIT photometry of Cl 0024+1654 and 3C 295.
o	Table 1: <BOI Cl 0024+1654 NNN> N=136, Table 2: <BOI 3C 295 NNN> N=107
Origin	of the Acronym: L (1983ApJS...52..183B)
Details on Acronym: Bok
Bok	(Bok+)
Write:	<<Bok R NNNA>>
N:	273+432+328+50+71
Object:	* (SIMBAD class: Star)
Note:	Tables 2 to 7: stars in regions (Nos I to V) In region I, format 'NNNB', B for stars with V < 14.50, format 'NNNF', F for stars with V ≥ 14.50 Identif. charts on Plates I to VI Only stars in region I (with 1950 coordinates) are available at CDS in electronic form.
Ref:	=1964MmMtS..16....0B
by	BOK B.J. , BASINSKI J.
	Mem. Mount Stromlo Obs., -1-None (1964)
	Stellar Distribution Near the South Galactic Pole, Photographic V Magnitudes and (B-V) Colours of 640 Stars in Region I.
o	Catalogue only for objects 'Bok I'
o	Table 2: <Bok I NNNB> N=271 among (Nos 1B-273B). Table 3: <Bok I NNNF> N=369 among (Nos 1F-432F). Table 4: <Bok II NNN> (Nos 1-328). Table 5: <Bok III NNN> (Nos 1-294). Table 6: <Bok IV NN> (Nos 1-50). Table 7: <Bok V NN> (Nos 1-71).
=E=	Catalogue in electronic form as II/119
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Bok
Bok	(Discoverer's name)= Ann. Bok
N:	1
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Ref:	=1977PASP...89..554P
by	PHILIP A.G.D. , DEMARQUE P., SWEIGART A.V., CIARDULLO R.B.
	Publ. Astron. Soc. Pac., 89, 554-556 (1977)
	A comparison of observations with main-sequence evolutionary models.
o	<NAME Bok OCl>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BoKa
BoKa	(Borngen+Kalloghlian)
Write:	<<BoKa NNN>>
N:	131
Object:	G (SIMBAD class: Galaxy)
Note:	N=131 G identified around the cluster ACO 2255. Identif. charts.
Ref:	=1979Afz....15..393B
by	BORNGEN F. , KALLOGHLIAN A.T.
	Astrofizika, 15, 393-400 (1979)
	Compact galaxies in the vicinity of the cluster A 2255.
o	<BoKa NNN> N=131
Origin	of the Acronym: L (1985AN....306...81B)
Details on Acronym: BoKar
BoKar	(Borngen+Karchentseva)
*****	Avoid the usage of BoKar, prefer BK
Origin	of the Acronym: L (1984AN....305...53B)
Details on Acronym: BOKS
BOKS	(Burrell Optical Kepler Survey)
Write:	<<BOKS NNNNN>>
N:	2460
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	KPNO Case Western Reserve University 0.61m Burrell Schmidt telescope observations of a field within the Kepler field of view.
Ref:	=2011AJ....142....2F
by	FELDMEIER J.J. , HOWELL S.B., SHERRY W., VON BRAUN K., EVERETT M.E., CIARDI D.R., HARDING P., MIHOS J.C., RUDICK C.S., LEE T.-H., KUTSKO R.M., VAN BELLE G.T.
	Astron. J., 142, 2 (2011)
	The Burrell-Optical-Kepler-Survey (BOKS). I. Survey description and initial results.
o	Tables 2-4: <BOKS NNNNN> N=1681+776+3 among (Nos 413-55937).
=E=	Catalogue in electronic form as <J/AJ/142/2/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Bol
Bol	(Bologna obs.)= (B) = (Ba87) = (Bo) = (N)
Write:	<<Bol NNN>>
N:	530
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Note:	Bologna observatory search for globular clusters in M 31.
in source:	M 31 = NGC 224
Ref:	=1980A&AS...42..357B
by	BATTISTINI P. , BONOLI F., BRACCESI A., FUSI PECCI F., MALAGNINI M.L., MARANO B.
	Astron. Astrophys., Suppl. Ser., 42, 357-374 (1980)
	Search for (globular) clusters in M 31. I. Candidates in a 70'square field centered on M 31.
o	Finding charts
o	Table III: <Bol NNN> (Nos 1-288), Table V: <Bol DNNN> (Nos D1-D132)
Ref:	=1987A&AS...67..447B
by	BATTISTINI P. , BONOLI F., BRACCESI A., FEDERICI L., FUSI PECCI F., MARANO B., BOERNGEN F.
	Astron. Astrophys., Suppl. Ser., 67, 447-482 (1987)
	Search for (globular) clusters in M 31. IV. Candidates in a 3x3° square field centered on M 31.
o	Table IV, col(1): The ID CMMSSDDMMm is not used in SIMBAD.
o	Table IV, col(1): <C MMSSDDMMm> N=113. Tables IV, V: <Bol NNN> (Nos 289-513, Nos 334 and 359 missing). Table VI: <Bol DNNN> (Nos D133-D350).
Ref:	=2005A&A...436..535G
by	GALLETI S. , BELLAZZINI M., FEDERICI L., FUSI PECCI F.
	Astron. Astrophys., 436, 535-540 (2005)
	The outermost cluster of M31.
o	Paragr.3: <Bol NNN> (No. 514) added.
Ref:	=2006A&A...456..985G
by	GALLETI S. , FEDERICI L., BELLAZZINI M., BUZZONI A., FUSI PECCI F.
	Astron. Astrophys., 456, 985-999 (2006)
	An updated survey of globular clusters in M 31. I. Classification and radial velocity for 76 candidate clusters.
o	Fig.10: <Bol NNN> (No. 515) added.
Ref:	=2007A&A...471..127G
by	GALLETI S. , BELLAZZINI M., FEDERICI L., BUZZONI A., FUSI PECCI F.
	Astron. Astrophys., 471, 127-136 (2007)
	An updated survey of globular clusters in M 31. II. Newly discovered bright and remote clusters.
o	Table m31rbc.dat: <RBC NNNN> N=1983 among (Nos 1-7737). Tables 3, B1, text: <Bol NNN> (Nos 516-524) added.
Ref:	=2007A&A...476..193B
by	BECCARI G. , BELLAZZINI M., CLEMENTINI G., FEDERICI L., FUSI PECCI F., GALLETI S., MONTEGRIFFO P., GIALLONGO E., RAGAZZONI R., GRAZIAN A., BARUFFOLO A., DE SANTIS C., DIOLAITI E., DI PAOLA A., FARINATO J., FONTANA A., GALLOZZI S., GASPARO F., GENTILE G., GREEN R., HILL J., KUHN O., MENCI N., PASIAN F., PEDICHINI F., SMAREGLIA R., SPEZIALI R., TESTA V., THOMPSON D., VERNET E., WAGNER R.M.
	Astron. Astrophys., 476, 193-198 (2007)
	A near-ultraviolet view of the inner region of M 31 with the large binocular telescope.
o	Table 1: <Bol NNN> (Nos 525-530) added.
=E=	Catalogue in electronic form as J/A+A/471/127
=E=	Catalogue in electronic form as <V/143/>
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Bol
Bol	(Bologna obs.)= (Bo) = (BolD) = (N)
Write:	<<Bol DNNN>>
N:	350
Object:	Misc. Obj. (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Note:	Table V in the first ref., Table VI in the second ref.. format 'DNNN': miscellaneous obj. of class D, not GCl.
in source:	M 31 = NGC 224
Ref:	=1980A&AS...42..357B
by	BATTISTINI P. , BONOLI F., BRACCESI A., FUSI PECCI F., MALAGNINI M.L., MARANO B.
	Astron. Astrophys., Suppl. Ser., 42, 357-374 (1980)
	Search for (globular) clusters in M 31. I. Candidates in a 70'square field centered on M 31.
o	Finding charts
o	Table III: <Bol NNN> (Nos 1-288), Table V: <Bol DNNN> (Nos D1-D132)
Ref:	=1987A&AS...67..447B
by	BATTISTINI P. , BONOLI F., BRACCESI A., FEDERICI L., FUSI PECCI F., MARANO B., BOERNGEN F.
	Astron. Astrophys., Suppl. Ser., 67, 447-482 (1987)
	Search for (globular) clusters in M 31. IV. Candidates in a 3x3° square field centered on M 31.
o	Table IV, col(1): The ID CMMSSDDMMm is not used in SIMBAD.
o	Table IV, col(1): <C MMSSDDMMm> N=113. Tables IV, V: <Bol NNN> (Nos 289-513, Nos 334 and 359 missing). Table VI: <Bol DNNN> (Nos D133-D350).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Bol
Bol	(Boller)
*****	Avoid the usage of Bol, prefer Boller
Origin	of the Acronym: L (Veron)
Details on Acronym: [BOL2016]
[BOL2016]	(Bouwens+Oesch+Labbe+, 2016)
Write:	<<[BOL2016] AAA910-NN>>
N:	47
Object:	Poss. G (SIMBAD class: Galaxy_Candidate = Galaxy Candidate)
Stat.	in SIMBAD: Ref. 2016ApJ...830...67B is completely incorporated.
Note:	N=47 galaxy candidates at z∼9-10 within the CANDELS-UDS, COSMOS, and EGS fields, pre-selected from the full HST, Spitzer IRAC S-CANDELS observations, and the deepest-available ground-based optical+near-infrared observations (CFHTLS-DEEP + HUGS + UltraVISTA + ZFOURGE).
in source:	NAME COSMOS Field
in source:	NAME Extended Groth Strip
in source:	NAME Hubble Ultra Deep Field
Ref:	=2016ApJ...830...67B
by	BOUWENS R.J. , OESCH P.A., LABBE I., ILLINGWORTH G.D., FAZIO G.G., COE D., HOLWERDA B., SMIT R., STEFANON M., VAN DOKKUM P.G., TRENTI M., ASHBY M.L.N., HUANG J.-S., SPITLER L., STRAATMAN C., BRADLEY L., MAGEE D.
	Astrophys. J., 830, 67-67 (2016)
	The bright end of the z ~ 9 and z ~ 10 UV luminosity functions using all five CANDELS fields.
o	Table 3: <[BOL2016] COS910-N> (Nos 0-4), <[BOL2016] UDS910-N> (Nos 0-4), <[BOL2016] EGS910-N> (Nos 0-7). Table 4: <[OBI2014] GN-z10-N> N=2 (Nos GN-z10-2 to GN-z10-3) added, <[OBI2014] GS-z9-N> N=4 (Nos GS-z9-2 to GS-z9-5) added.
Ref:	=2019ApJ...880...25B
by	BOUWENS R.J. , STEFANON M., OESCH P.A., ILLINGWORTH G.D., NANAYAKKARA T., ROBERTS-BORSANI G., LABBE I., SMIT R.
	Astrophys. J., 880, 25-25 (2019)
	Newly discovered bright z ~ 9-10 galaxies and improved constraints on their prevalence using the full CANDELS area.
o	In table 5, UDS910-5 is probably erroneous, the coordinates don't match the ones given in tables 1 and 2 used in SIMBAD.
o	Tables 1+2+4+5: <[BOL2016] COS910-NN> (Nos 5-12) added, <[BOL2016] EGS910-NN> (Nos 8-18) added, <[BOL2016] UDS910-NN> (Nos 5-14) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BolD
BolD	(Bologna obs., field D)
*****	Avoid the usage of BolD, prefer Bol
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Boller
Boller	(Boller)= (Bol)
Write:	<<Boller NNN>> <<Boller NNN.N>>
N:	254
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	1989AN....310..187B: N=6 QSO Nos 75, 105, 121.1, 131, 140, 192, belonging to the list of N=254 objects of Boller Thesis.
Ref:	=1989AN....310..187B
by	BOLLER T. , LORENZ H., AFANAS'EV V.L., DODONOV S.N., TEREBIZH V.Y.
	Astron. Nachr., 310, 187-193 (1989)
	On the cosmological evolution of the quasar population.
o	Table 4: <Boller NNN> N=6 among 254. Fig.2: <[BJK80] N> Nos 5, 6 are new
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Bolo
Bolo	(Bolometer camera)
*****	Avoid the usage of Bolo, prefer [EGE2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Bolo
Bolo	(Bolometer camera)
*****	Avoid the usage of Bolo, prefer [EYG2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Bolo
Bolo	(Bolometer camera)
*****	Avoid the usage of Bolo, prefer [YEE2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Bolocam-LE1100
Bolocam-LE1100	(Bolometer Camera, Lockman East, 1100mu.m)= (LE1100)
Write:	<<Bolocam-LE1100 NN>>
N:	17
Object:	G candidate (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	1.1mm survey of the East of the Lockman Hole, using Bolocam at CSO.
in source:	NAME Lockman Hole
Ref:	=2005ApJ...623..742L
by	LAURENT G.T. , AGUIRRE J.E., GLENN J., ADE P.A.R., BOCK J.J., EDGINGTON S.F., GOLDIN A., GOLWALA S.R., HAIG D., LANGE A.E., MALONEY P.R., MAUSKOPF P.D., NGUYEN H., ROSSINOT P., SAYERS J., STOVER P.
	Astrophys. J., 623, 742-762 (2005)
	The Bolocam Lockman hole millimeter-wave galaxy survey: galaxy candidates and number counts.
o	Table 2, text: <Bolocam-LE1100 NN> (Nos 1-17).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BOM2000]
[BOM2000]	(Bally+O'Dell+McCaughrean, 2000)
Write:	<<[BOM2000] {d\|j\|w}SSs-MSS>> <<[BOM2000] {d\|j\|w}SSs-MMSS>> <<[BOM2000] LL Ori WNa>>
N:	48+23+10+7
Object:	Feature (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST WFPC2 observations of Orion Nebula. In the format 'SSs-MSS' and 'SSs-MMSS', offset relative to: 5h35m and -5deg20'. Format 'dSSs-MSS' and 'dSSs-MMSS', disks (letter'd') seen only in silhouette sometimes embedded with bright proplyds. Format 'jSSs-MSS', microjets (letter 'j') and bipolar outflows. Format 'wSSs-MSS', wind (letter 'w') collision fronts. Format 'LL Ori WNa', knots associated with LLOri bow. See also [BJJ2001b], [BR2001].
in source:	NAME Orion Nebula
Ref:	=2000AJ....119.2919B
by	BALLY J. , O'DELL C.R., McCAUGHREAN M.J.
	Astron. J., 119, 2919-2959 (2000)
	Disks, microjets, windblown bubbles, and outflows in the Orion nebula.
o	<HH NNN> (Nos 508-530). Tables 1, 2: <[BOM2000] dSSs-MSS>, <[BOM2000] dSSs-MMSS>, N=15+33. Table 3: <[BOM2000] jSSs-MSS> N=23. Table 4: <[BOM2000] wSSs-MSS> N=10, <[BOM2000] LL Ori WNa> (Nos N1-N3, S1-S3, N2a-N2b).
Ref:	=2005AJ....129..382S
by	SMITH N. , BALLY J., LICHT D., WALAWENDER J.
	Astron. J., 129, 382-392 (2005)
	New silhouette disks with reflection nebulae and outflows in the Orion nebula and M43.
o	Table 1: <[BOM2000] dSSs-MSS>, <[BOM2000] dSSs-MMSS>, N=9 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Boo
Boo	(Bootes I) (Not yet in Simbad)
*****	Avoid the usage of Boo, prefer [NGW2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Bootes
Bootes	(Brand+Weedman+Desai+, 2008)
*****	Avoid the usage of Bootes, prefer [BWD2008b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 70Bootes
70Bootes	(70mu.m, Bootes)
*****	Avoid the usage of 70Bootes, prefer [BWD2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Bor-AC
Bor-AC	(Bordeaux Astrographic Catalogue)
*****	Avoid the usage of Bor-AC, prefer BAC
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BoRG
BoRG	(Brightest of Reionizing Galaxies)
Write:	<<BoRG NN NNNN+NNNN>> <<BoRG Na NNNN+NNNN>> <<BoRG NNNN+NNNN NNNN>>
N:	2+6+37
Object:	G (SIMBAD class: Galaxy)
Note:	The Brightest of Reionizing Galaxies (BoRG) Survey is a large Hubble Space Telescope Program focused on finding rare and bright galaxy candidates at redshift z∼8. Over 50 fields have been acquired with WFC3 in four bands for a total area exceeding 250arcmin2. See also the website: https://wolf359.colorado.edu/
Ref:	=2011ApJ...727L..39T
by	TRENTI M. , BRADLEY L.D., STIAVELLI M., OESCH P., TREU T., BOUWENS R.J., SHULL J.M., MacKENTY J.W., CAROLLO C.M., ILLINGWORTH G.D.
	Astrophys. J., 727L, 39 (2011)
	The Brightest of Reionizing Galaxies survey: design and preliminary results.
o	Table 2: <BoRG NN NNNN+NNNN> N=2, <BoRG Na NNNN+NNNN> N=2.
Ref:	=2012ApJ...746...55T
by	TRENTI M. , BRADLEY L.D., STIAVELLI M., SHULL J.M., OESCH P., BOUWENS R.J., MUNOZ J.A., ROMANO-DIAZ E., TREU T., SHLOSMAN I., CAROLLO C.M.
	Astrophys. J., 746, 55 (2012)
	Overdensities of y-dropout galaxies from the Brightest-of-Reionizing galaxies survey: a candidate protocluster at redshift z ~ 8.
o	Table 1: <[TBS2012] DDD.dddd+DD.dddd> N=21. Table 2: <BoRG 58 NNNN+NNNN> N=5.
Ref:	=2012ApJ...760..108B
by	BRADLEY L.D. , TRENTI M., OESCH P.A., STIAVELLI M., TREU T., BOUWENS R.J., SHULL J.M., HOLWERDA B.W., PIRZKAL N.
	Astrophys. J., 760, 108 (2012)
	The Brightest of Reionizing Galaxies survey: constraints on the bright end of the z ~ 8 luminosity function.
o	Tables 3-6: <BoRG HHMM+DDMM NNNN> N=8+25+5+2.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Borngen
Borngen	(Borngen)= (Bo)
Write:	<<Borngen NNN>>
N:	205
Object:	Faint Blue Obj. (SIMBAD class: blue = Blue Object)
Stat:	is completely incorporated in Simbad
Note:	1st ref., Borngen, 1980: (Nos 1-95). 2nd ref.: Faint blue galaxies (Nos 96-205)
Ref:	=1980AN....301..305B
by	BORNGEN F.
	Astron. Nachr., 301, 305-310 (1980)
	Very faint blue objects in the Virgo cluster region.
o	<Borngen NN> (Nos 1-95)
Ref:	=1984AN....305...41B
by	BORNGEN F.
	Astron. Nachr., 305, 41-44 (1984)
	Faint blue galaxies in the Virgo cluster region.
o	<Borngen NNN> (Nos 96-205)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BOS2021]
[BOS2021]	(Bouwens+Oesch+Stefanon+, 2021) (Not yet in Simbad)
Write:	<<[BOS2021] HUDF-MSSssMMSSs>> <<[BOS2021] HDUVW275-MSSssMMSSs>> <<[BOS2021] HDUVW336-MSSssMMSSs>> <<[BOS2021] ANNNNPA-MSSssMMSSs>> <<[BOS2021] AS1063PA-MSSssMMSSs>> <<[BOS2021] MHHMMPA-MSSssMMSSs>>
N:	1069+3858+7171+1094+379+1113
Object:	G (SIMBAD class: Galaxy)
Note:	Galaxies in noncluster extragalactic legacy fields, including the Hubble Ultra Deep Field, the Hubble Frontier Fields parallel fields, and all five CANDELS fields. Use of HST data (HDUV, UVUDF, HFF, HUDF).
Ref:	=2021AJ....162...47B
by	BOUWENS R.J. , OESCH P.A., STEFANON M., ILLINGWORTH G., LABBE I., REDDY N., ATEK H., MONTES M., NAIDU R., NANAYAKKARA T., NELSON E., WILKINS S.
	Astron. J., 162, 47-47 (2021)
	New determinations of the UV luminosity functions from z ~ 9 to 2 show a remarkable consistency with halo growth and a constant star formation efficiency.
o	Table 2: <[BOS2021] HUDF-MSSssMMSSs> N=1069, <[BOS2021] HDUVW275-MSSssMMSSs> N=3858, <[BOS2021] HDUVW336-MSSssMMSSs> N=7171, <[BOS2021] ANNNNPA-MSSssMMSSs> N=1094, <[BOS2021] AS1063PA-MSSssMMSSs> N=379, <[BOS2021] MHHMMPA-MSSssMMSSs> N=1113.
=E=	Catalogue in electronic form as <J/AJ/162/47/>
Details on Acronym: Boss
Boss	(Boss)
*****	Avoid the usage of Boss, prefer [B10]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Boss
Boss	(Boss)
====>	Equivalent to: GC
Details on Acronym: BOW
BOW	(Butcher+Oemler+Wells)= (BO)
Write:	<<BOW ACO NNNN AANNNa>> <<BOW Cl HHMM+DDMM NNN>>
N:	about 6000
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	In the format, 'AANNN' stands for: 'CCNNN' in each ACO Cluster Center, 'BFNNN' in each Blank Field corresponding to an ACO. In 1998ApJ...508L.139B, the authors found 2 galaxies 'ACO 370 CC24', and refer to them as 24a and 24b. For Cl clusters the format is 'NNN', without distinguishing center and blank field.
Ref:	=1983ApJS...52..183B
by	BUTCHER H. , OEMLER A., WELLS D.C.
	Astrophys. J., Suppl. Ser., 52, 183-228 (1983)
	The evolution of galaxies in clusters. III. Photometry of 17 intermediate redshift clusters.
o	<BOW ACO NNNN CCNNN> (CC for Cluster Center) <BOW ACO NNNN BFNNN> (BF for Blank Field) <BOW Cl HHMM+DDMM NNN> N about 6000
Ref:	=1998ApJ...508L.139B
by	BROWN T.M. , FERGUSON H.C., DEHARVENG J.-M., JEDRZEJEWSKI R.I.
	Astrophys. J., 508, 139-142 (1998)
	Measurements of Far-UV emission from elliptical galaxies at z = 0.375.
o	Table 2: <BOW ACO 370 CCNNa> (Nos CC24a, 24b, 34a).
Origin	of the Acronym: L (1991A&AS...91....1P)
Details on Acronym: BP
BP	(Bailey+Pooley)
Write:	<<BP NNN>>
N:	198
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Ref:	=1968MNRAS.138...51B
by	BAILEY J.A. , POOLEY G.G.
	Mon. Not. R. Astron. Soc., 138, 51-66 (1968)
	Fan-beam observations of radio sources at 408 and 1407 MHz.
o	Table I: <BP NNN> (Nos 1-198)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BP2001]
[BP2001]	(Bernabei+Polcaro, 2001)
Write:	<<[BP2001] NN>>
N:	75
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	NAME Loiano 1
Ref:	=2001A&A...371..123B
by	BERNABEI S. , POLCARO V.F.
	Astron. Astrophys., 371, 123-132 (2001)
	A search for peculiar objects in young open clusters. II. A new Be star, the optical counterpart of IRAS 19564+3224 and a new open cluster in Vulpecula.
o	in ref list FABREGAT J., REGLERO V., 1990MNRAS.247..407F instead of 249.414
o	<NAME LOIANO 1>. p.126: <Cl* NGC 6871 BP NN> (No. 10) added. Table 3: <[BP2001] NN> (Nos 1-75).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BP98]
[BP98]	(Bazell+Peng, 1998) (Not yet in Simbad)
Write:	<<[BP98] NN>>
N:	87
Object:	G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Ref:	=1998ApJS..116...47B
by	BAZELL D. , PENG Y.
	Astrophys. J., Suppl. Ser., 116, 47-55 (1998)
	A comparison of neural network algorithms and preprocessing methods for star-galaxy discrimination.
o	Table 1: objects not in SIMBAD.
o	Table 1: <[BP98] NN> (Nos 1-87)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPA2013]
[BPA2013]	(Bussmann+Perez-Fournon+Amber+, 2013)
Write:	<<[BPA2013] H-ATLAS JHHMMSS.s+DDMMSS lens>> <<[BPA2013] H-ATLAS J083051.0+013224 lens N>>
N:	6+2
Object:	Grav. lens (SIMBAD class: GravLens = Gravitational Lens)
Stat:	is completely incorporated in Simbad
Note:	Gravitational lensing of SMGs in the HerMES and H-ATLAS surveys. SMA high-spatial resolution imaging. Gemini-South and MMT optical spectroscopy.
Ref:	=2013ApJ...779...25B
by	BUSSMANN R.S. , PEREZ-FOURNON I., AMBER S., CALANOG J., GURWELL M.A., DANNERBAUER H., DE BERNARDIS F., FU H., HARRIS A.I., KRIPS M., LAPI A., MAIOLINO R., OMONT A., RIECHERS D., WARDLOW J., BAKER A.J., BIRKINSHAW M., BOCK J., BOURNE N., CLEMENTS D.L., COORAY A., DE ZOTTI G., DUNNE L., DYE S., EALES S., FARRAH D., GAVAZZI R., GONZALEZ NUEVO J., HOPWOOD R., IBAR E., IVISON R.J., LAPORTE N., MADDOX S., MARTINEZ-NAVAJAS P., MICHALOWSKI M., NEGRELLO M., OLIVER S.J., ROSEBOOM I.G., SCOTT D., SERJEANT S., SMITH A.J., SMITH M., STREBLYANSKA A., VALIANTE E., VAN DER WERF P., VERMA A., VIEIRA J.D., WANG L., WILNER D.
	Astrophys. J., 779, 25 (2013)
	Gravitational lens models based on Submillimeter Array imaging of Herschel-selected strongly lensed sub-millimeter galaxies at z > 1.5.
o	Table 1: <[BPA2013] H-ATLAS JHHMMSS.s+DDMMSS lens> N=6, <[BPA2013] H-ATLAS J083051.0+013224 lens N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPA2014]
[BPA2014]	(Bogdanov+Patruno+Archibald+, 2014)
Write:	<<[BPA2014] J122807.5-485324>> <<[BPA2014] J122807.427-485323.561>>
N:	2
Object:	Cluster of G + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton, Chandra, and VLT/FORS2 observations of N=1 galaxy cluster, with its likely central galaxy, in the field of XSS J12270-4859.
Ref:	=2014ApJ...789...40B
by	BOGDANOV S. , PATRUNO A., ARCHIBALD A.M., BASSA C., HESSELS J.W.T., JANSSEN G.H., STAPPERS B.W.
	Astrophys. J., 789, 40 (2014)
	X-ray observations of XSS J12270-4859 in a new low state: a transformation to a disk-free rotation-powered pulsar binary.
o	<[BPA2014] J122807.5-485324> N=1. <[BPA2014] J122807.427-485323.561> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPB2005]
[BPB2005]	(Bedin+Piotto+Baume+, 2005)= (B)
Write:	<<[BPB2005] NNN>>
N:	110
Object:	Cluster of * + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Study of M 33 based on WFC-ACS images from the HST archives: 33 star clusters, 51 candidates, and 26 micellaneous objects are found.
in source:	M 33 = NGC 598
Ref:	=2005A&A...444..831B
by	BEDIN L.R. , PIOTTO G., BAUME G., MOMANY Y., CARRARO G., ANDERSON J., MESSINEO M., ORTOLANI S.
	Astron. Astrophys., 444, 831-836 (2005)
	Star cluster detection with WFC/ACS in M33. 33 new clusters and 51 candidates.
o	Tables 1, 2, 3: <[BPB2005] NNN> (Nos 1-33, 34-57, 58-110).
=E=	Catalogue in electronic form as J/A+A/444/831
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPB2009]
[BPB2009]	(Braglia+Pierini+Biviano+, 2009)
Write:	<<[BPB2009] A2744 NNNNN>> <<[BPB2009] A2537 NNNNN>>
N:	395+809
Object:	G (SIMBAD class: Galaxy)
Note:	VLT VIMOS spectroscopy, ESO/MPG 2.2m telescope WFI and GALEX photometry of X-ray luminous galaxy clusters.
in source:	ACO 2744 = ACCG 118
in source:	ACO 2537
Ref:	=2009A&A...500..947B
by	BRAGLIA F.G. , PIERINI D., BIVIANO A., BOEHRINGER H.
	Astron. Astrophys., 500, 947-963 (2009)
	Multi-wavelength study of X-ray luminous clusters at z ~ 0.3. I. Star-formation activity of cluster galaxies.
o	Table 9: <[BPB2009] A2744 NNNNN> N=395 among (Nos 5246-22734). Table 10: <[BPB2009] A2537 NNNNN> N=809 among (Nos 3011-14816).
=E=	Catalogue in electronic form as <J/A+A/500/947/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPB2012]
[BPB2012]	(Benedettini+Pezzuto+Burton+, 2013)
Write:	<<[BPB2012] LupN CN>>
N:	15
Object:	Dense Core (SIMBAD class: denseCore = Dense Core)
Note:	Mopra telescope 3mm and 12mm line observations of N=15 dense cores in the molecular clouds Lupus 1, 3 and 4.
in source:	NAME Lupus I = Lupus 1
in source:	NAME Lupus III = Lupus 3
in source:	NAME Lupus IV = Lupus 4
Ref:	=2012MNRAS.419..238B
by	BENEDETTINI M. , PEZZUTO S., BURTON M.G., VITI S., MOLINARI S., CASELLI P., TESTI L.
	Mon. Not. R. Astron. Soc., 419, 238-250 (2012)
	Multiline spectral imaging of dense cores in the Lupus molecular cloud.
o	Table 2: <[BPB2012] Lup1 CN> (Nos C1-C8), <[BPB2012] Lup3 CN> (Nos C1-C5), <[BPB2012] Lup4 CN> (Nos C1-C2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPB98]
[BPB98]	(Bowen+Pettini+Boyle, 1998)
Write:	<<[BPB98] NNN>>
N:	84
Object:	G (SIMBAD class: Galaxy)
Note:	Table 1: N=84 galaxies among (Nos 1-347) in the field of QSO 1821+643. 'Ext' indicate objects which were not selected from the APM scans as galaxies, but were nevertheless added because of their classifications as galaxies or because of their proximity to the QSO sightline. They turned out to be stars.
Ref:	=1998MNRAS.297..239B
by	BOWEN D.V. , PETTINI M., BOYLE B.J.
	Mon. Not. R. Astron. Soc., 297, 239-250 (1998)
	Ly-α absorption in the nearby Universe: the sightline to Q1821+643.
o	Table 1: 'Ext' not in SIMBAD. Table 2: Ly-α systems not in SIMBAD.
o	Table 1: <[BPB98] NNN> N=84 among (Nos 1-347)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BPC
BPC	(Buta+Purcell+Crocker)
*****	Avoid the usage of BPC, prefer [BPC95]
Origin	of the Acronym: L (1999AJ....118.2071B)
Details on Acronym: [BPC2003]
[BPC2003]	(Beswick+Pedlar+Clemens+, 2003)
Write:	<<[BPC2003] NN>>
N:	10
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	MERLIN observations at 1.4 GHz. N=10 nuclear components within NGC 520.
in source:	NGC 520
Ref:	=2003MNRAS.346..424B
by	BESWICK R.J. , PEDLAR A., CLEMENS M.S., ALEXANDER P.
	Mon. Not. R. Astron. Soc., 346, 424-432 (2003)
	A high-resolution radio study of neutral gas in the starburst galaxy NGC 520.
o	Tables 1, 2: <[BPC2003] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPC2006]
[BPC2006]	(Berger+Penprase+Cenko+, 2006)
Write:	<<[BPC2006] GRB 050505 abs N.NNNN>>
N:	3
Object:	Absorber
Note:	Optical spectroscopy of GRB 050505 with the LRIS on Keck I: 3 redshift sytems are observed in the spectrum.
Ref:	=2006ApJ...642..979B
by	BERGER E. , PENPRASE B.E., CENKO S.B., KULKARNI S.R., FOX D.B., STEIDEL C.C., REDDY N.A.
	Astrophys. J., 642, 979-988 (2006)
	Spectroscopy of GRB 050505 at z = 4.275: a logN(H i) = 22.1 DLA host galaxy and the nature of the progenitor.
o	Fig.2: <[BPC2006] GRB 050505 abs N.NNNN> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPC2019]
[BPC2019]	(Barro+Perez-Gonzalez+Cava+, 2019)
Write:	<<[BPC2019] NNNNN>>
N:	35445
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	A multiwavelength photometric catalog of N=35445 F160W-selected sources in the GOODS-North field as part of the observations by the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS). See also CANDELS GDN.
in source:	NAME GOODS North Field
Ref:	=2019ApJS..243...22B
by	BARRO G. , PEREZ-GONZALEZ P.G., CAVA A., BRAMMER G., PANDYA V., ELICHE MORAL C., ESQUEJ P., DOMINGUEZ-SANCHEZ H., ALCALDE PAMPLIEGA B., GUO Y., KOEKEMOER A.M., TRUMP J.R., ASHBY M.L.N., CARDIEL N., CASTELLANO M., CONSELICE C.J., DICKINSON M.E., DOLCH T., DONLEY J.L., BRIONES N.E., FABER S.M., FAZIO G.G., FERGUSON H., FINKELSTEIN S., FONTANA A., GALAMETZ A., GARDNER J.P., GAWISER E., GIAVALISCO M., GRAZIAN A., GROGIN N.A., HATHI N.P., HEMMATI S., HERNAN-CABALLERO A., KOCEVSKI D., KOO D.C., KODRA D., LEE K.-S., LIN L., LUCAS R.A., MOBASHER B., McGRATH E.J., NANDRA K., NAYYERI H., NEWMAN J.A., PFORR J., PETH M., RAFELSKI M., RODRIGUEZ-MUNOZ L., SALVATO M., STEFANON M., VAN DER WEL A., WILLNER S.P., WIKLIND T., WUYTS S.
	Astrophys. J., Suppl. Ser., 243, 22-22 (2019)
	The CANDELS/SHARDS multiwavelength catalog in GOODS-N: photometry, photometric redshifts, stellar masses, emission-line fluxes, and star formation rates.
o	<CANDELS GDN JHHMMSS.s+DDMMMSS.s> N=35445 = <[BPC2019] NNNNN> N=35445 among (Nos 1-35451).
=E=	Catalogue in electronic form as <J/ApJS/243/22/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPC95]
[BPC95]	(Buta+Purcell+Crocker, 1995)= (BPC)
Write:	<<[BPC95] NN>>
N:	51
Object:	HII (SIMBAD class: HIIReg = HII Region)
in source:	ESO 565-11
Ref:	=1995AJ....110.1588B
by	BUTA R. , PURCELL G.B., CROCKER D.A.
	Astron. J., 110, 1588-1601 (1995)
	Intrinsic bar/ring misalignment and a starburst nuclear ring in the peculiar spiral galaxy ESO 565-11.
o	(Erratum) Erratum 1995, AJ 110, p. 1588 + 1996, AJ 111, p. 983
o	Table 7: <[BPC95] NN> (Nos 1-51)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPC97]
[BPC97]	(Butler+Piro+Costa, 1997)
Write:	<<[BPC97] source a>> <<[BPC97] source N>>
N:	2+3
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	BeppoSAX and ROSAT observations of GRB 970111 field.
Ref:	=1997IAUC.6539Q...1B
by	BUTLER R.C. , PIRO L., COSTA E., FEROCI M., FRONTERA F., DAL FIUME D., HEISE J., JAGER R., SACCO B., CHIAPPETTI L., PARMAR A., ANTONELLI L.A., RICCI D., MULLER J.M., COLETTA A., DE LIBERO C., SALOTTI L., VOGES W., BOLLER T., GREINER J.
	IAU Circ., 6539, 1-None (1997)
	GRB 970111.
o	<[BPC97] source a> (Nos a-b), <[BPC97] source N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPC99]
[BPC99]	(Bergeron+Petitjean+Cristiani+, 1999)
Write:	<<[BPC99] GN>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST STIS observations on the VLT N=3 galaxies in the field of the QSO '[SDW98] J2233-606', in the HDFS Map in Fig.2.
in source:	NAME HDFS
Ref:	=1999A&A...343L..40B
by	BERGERON J. , PETITJEAN P., CRISTIANI S., ARNOUTS S., BRESOLIN F., FASANO G.
	Astron. Astrophys., 343, 40-44 (1999)
	Lyα emission at z~z_<EM> around the quasar J2233-606 in the Hubble Deep Field South.
o	Quasar J2233-606 is [SDW98] J2233-606 in SIMBAD
o	Table 1: <[BPC99] GN> (Nos G1-G3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPE2009]
[BPE2009]	(Busquet+Palau+Estalella+, 2009)
Write:	<<[BPE2009] MMN>> <<[BPE2009] VLA NN>> <<[BPE2009] VLA NA>> <<[BPE2009] IRS 1>> <<[BPE2009] SC>>
N:	2+12+2+1+1
Object:	(mm) + (Rad) + (IR) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	VLA 6cm, 3.6cm, 1.3cm, and 0.7cm continuum and IRAM 30m 1.2mm continuum observations of the field of IRAS 00213+6530.
Ref:	=2009A&A...506.1183B
by	BUSQUET G. , PALAU A., ESTALELLA R., GIRART J.M., ANGLADA G., SEPULVEDA I.
	Astron. Astrophys., 506, 1183-1198 (2009)
	Low-mass protostars and dense cores in different evolutionary stages in IRAS 00213+6530.
o	Table 2: <[BPE2009] MMN> (Nos MM1-MM2). Table 3: <[BPE2009] VLA NN> (Nos VLA 1-VLA 12). Table 5: <[BPE2009] VLA NA> (Nos VLA 8A-VLA 8B). Table 6: <[BPE2009] IRS 1>, <[BPE2009] SC>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPG2011]
[BPG2011]	(Barro+Perez-Gonzales+Gallego+, 2011)= ([BPG2011a]) = (irac)
Write:	<<[BPG2011] iracNNNNNN>> <<[BPG2011] iracNNNNNN N>> <<[BPG2011] iracNNNNNN_N>> (not recognised by Simbad, but found in literature)
N:	76396
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	IRAC 3.6+4.5mu.m selected catalog in the Extended Groth Strip (EGS). Use of data from Chandra ACIS, GALEX, CFHT MegaCam, MMT Megacam, HST ACS and NICMOS, Subaru Suprime-Cam and MOIRCS, Palomar and Calar Alto, Spitzer IRAC and MIPS, VLA, Keck DEIMOS observations.
in source:	NAME Extended Groth Strip
Ref:	=2011ApJS..193...13B
by	BARRO G. , PEREZ-GONZALEZ P.G., GALLEGO J., ASHBY M.L.N., KAJISAWA M., MIYAZAKI S., VILLAR V., YAMADA T., ZAMORANO J.
	Astrophys. J., Suppl. Ser., 193, 13 (2011)
	UV-to-FIR analysis of Spitzer/IRAC sources in the Extended Groth Strip. I. Multi-wavelength photometry and spectral energy distributions.
o	Tables 5-6: <[BPG2011] iracNNNNNN>, <[BPG2011] iracNNNNNN N> N=76396.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPG2011a]
[BPG2011a]	(Barro+Perez-Gonzales+Gallego+, 2011)
*****	Avoid the usage of [BPG2011a], prefer [BPG2011]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPG2011b]
[BPG2011b]	(Bellazzini+Perina+Galleti+, 2011)
Write:	<<[BPG2011b] NNNNN>>
N:	69795
Object:	* (SIMBAD class: Star)
Note:	VI photometry of N=69795 stars in the dwarf galaxy VV 124, obtained from archival HST ACS images.
in source:	VV 124 = UGC 4879
Ref:	=2011A&A...533A..37B
by	BELLAZZINI M. , PERINA S., GALLETI S., OOSTERLOO T.
	Astron. Astrophys., 533A, 37-37 (2011)
	HST-ACS photometry of the isolated dwarf galaxy VV124=UGC 4879. Detection of the blue horizontal branch and identification of two young star clusters.
o	Fig. 8, Table 4: <[BBO2011] CN> (No. C2) added. vv124: <[BPG2011b] NNNNN> N=69795 among (Nos 3-69872).
=E=	Catalogue in electronic form as J/A+A/533/A37
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BPGS
BPGS	(Bruzual+Persson+Gunn+Stryker)
*****	Avoid the usage of BPGS, prefer [GS83]
Origin	of the Acronym: L (2004ApJ...606..952R)
Details on Acronym: [BPH2004]
[BPH2004]	(Bassa+Pooley+Homer+, 2004)= (CX)
Write:	<<[BPH2004] CX NN>>
N:	31
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of M 4 cluster. Optical counterparts from HST archival data.
in source:	M 4 = NGC 6121
Ref:	=2004ApJ...609..755B
by	BASSA C. , POOLEY D., HOMER L., VERBUNT F., GAENSLER B.M., LEWIN W.H.G., ANDERSON S.F., MARGON B., KASPI V.M., VAN DER KLIS M.
	Astrophys. J., 609, 755-765 (2004)
	X-ray sources and their optical counterparts in the globular cluster M4.
o	(Erratum) Addendum vol. 619, p. 1189 (2005)
o	Table 1 : CX 9w is a misprint for CX 9
o	Table 1: <[BPH2004] CX NN> (Nos 1-31).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPH2019]
[BPH2019]	(Bhardwaj+Panwar+Herczeg+, 2019)
Write:	<<[BPH2019] V1NN>>
N:	95
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	Tenagra 0.81m telescope observations of N=95 variable stars towards the star-forming region Pelican Nebula.
in source:	IC 5070 = NAME Pelican Nebula
Ref:	=2019A&A...627A.135B
by	BHARDWAJ A. , PANWAR N., HERCZEG G.J., CHEN W.P., SINGH H.P.
	Astron. Astrophys., 627A, 135-135 (2019)
	Variability of young stellar objects in the star-forming region Pelican Nebula.
o	Tables 1-4: <[BPH2019] VNNN> (Nos V101-V195).
=E=	Catalogue in electronic form as <J/A+A/627/A135/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPJ2000]
[BPJ2000]	(Briggs+Pye+Jeffries+, 2000)
Write:	<<[BPJ2000] NGC 6633 NN>> <<[BPJ2000] IC 4756 NN>>
N:	32+13
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations of NGC 6633 and IC 4756. See also [RSS98] for IC 4756 observations.
in source:	NGC 6633
in source:	IC 4756
Ref:	=2000MNRAS.319..826B
by	BRIGGS K.R. , PYE J.P., JEFFRIES R.D., TOTTEN E.J.
	Mon. Not. R. Astron. Soc., 319, 826-836 (2000)
	X-ray source populations in the region of the open clusters NGC 6633 and IC 4756.
o	in ref list Heiles at al 1981ApJ.247L.73 instead of 73, Kopff 1943AN.274.69 instead of 93
o	Table 4: <[BPJ2000] NGC 6633 NN> (Nos 1-32). Table 5: <[BPJ2000] IC 4756 NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPK2003]
[BPK2003]	(Bedin+Piotto+King+, 2003)
Write:	<<[BPK2003] QSO>> <<[BPK2003] Star N>>
N:	1+3
Object:	QSO + * (SIMBAD class: QSO = Quasar)
Note:	HST WFPC2 observations of M 4. N=3 stars in the field of M 4 near an extragalactic source identified as a background QSO.
Ref:	=2003AJ....126..247B
by	BEDIN L.R. , PIOTTO G., KING I.R., ANDERSON J.
	Astron. J., 126, 247-254 (2003)
	Hubble Space Telescope astrometry of M4 and the galactic constant V_{0}/R{0}.
o	Fig.5: <[BPK2003] QSO> N=1, <[BPK2003] Star N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPL2020]
[BPL2020]	(Bidaran+Pasquali+Lisker+, 2020)
Write:	<<[BPL2020] BBN>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Note:	VLT MUSE observations of N=2 galaxies in the fields of VCC 1836 and VCC 170 respectively.
in source:	VCC 1836
in source:	VCC 170
Ref:	=2020MNRAS.497.1904B
by	BIDARAN B. , PASQUALI A., LISKER T., COCCATO L., FALCON-BARROSO J., VAN DE VEN G., PELETIER R., EMSELLEM E., GREBEL E.K., LA BARBERA F., JANZ J., SYBILSKA A., VIJAYARAGHAVAN R., GALLAGHER J., GADOTTI D.A.
	Mon. Not. R. Astron. Soc., 497, 1904-1924 (2020)
	On the accretion of a new group of galaxies on to Virgo: I. Internal kinematics of nine in-falling dEs.
o	Figs E1-E2, Table E1: <[BPL2020] BBN> (Nos BB1-BB2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPL98]
[BPL98]	(Bagchi+Pislar+Lima Neto, 1998)
Write:	<<[BPL98] VSSRS>> <<[BPL98] South Blob>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio relic VSSRS (Very Steep Spectrum Radio Source) in ACO 85 and 'South Blob'. Both are radio-source and X-ray source.
in source:	ACO 85
Ref:	=1998MNRAS.296L..23B
by	BAGCHI J. , PISLAR V., LIMA NETO G.B.
	Mon. Not. R. Astron. Soc., 296, 23-28 (1998)
	The diffuse, relic radio source in Abell 85: estimation of cluster-scale magnetic field from inverse Compton X-rays.
o	The seyfert galaxie = Ka 364.
o	<[BPL98] VSSRS> N=1, <[BPL98] South Blob> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BPM
BPM	(Bruce, Proper Motion survey)
Write:	<<BPM NNNNN>>
N:	98218
Object:	PM* (SIMBAD class: HighPM* = High Proper Motion Star)
Ref:	=1963BPM...C......0L
by	LUYTEN W.J.
	Bruce proper motion survey. The general catalogue (vol 1,2)., 0-None (1963)
	Bruce proper motion survey. The general catalogue. Vol. I, II.
o	<BPM NNNNN> (Nos 1-98218).
Details on Acronym: [BPM2001]
[BPM2001]	(Bocchino+Parmar+Mereghetti+, 2001)
Write:	<<[BPM2001] Src A>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	BeppoSAX Galactic Plane survey: N=3 X-ray sources (Nos A-C) within the radio shell of SNR 318.2+0.1.
Ref:	=2001A&A...367..629B
by	BOCCHINO F. , PARMAR A.N., MEREGHETTI S., ORLANDINI M., SANTANGELO A., ANGELINI L.
	Astron. Astrophys., 367, 629-634 (2001)
	X-ray emission in the direction of the SNR G318.2+0.1.
o	Fig.2, Table 1: <[BPM2001] Src A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPM2002]
[BPM2002]	(Beswick+Pedlar+McDonald, 2002)
Write:	<<[BPM2002] NGC 7469 A>> <<[BPM2002] NGC 7469 nucleus>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	MERLIN observations. Radio components of NGC 7469.
in source:	NGC 7469
Ref:	=2002MNRAS.335.1091B
by	BESWICK R.J. , PEDLAR A., McDONALD A.R.
	Mon. Not. R. Astron. Soc., 335, 1091-1099 (2002)
	Sub-arcsecond atomic hydrogen absorption in the Seyfert galaxies NGC 7674 and NGC 7469.
o	Table 1: radio components of NGC 7674 = [UPA88] NGC 7674 C, E, W. p.1098: PKS 1545-79 is a misprint for PKS 1549-79
o	Fig.4, Table 2: <[BPM2002] NGC 7469 A> (Nos A-C), <[BPM2002] NGC 7469 nucleus> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPM2022]
[BPM2022]	(Bhukta+Pal+Mondal, 2022)
Write:	<<[BPM2022] JHHMM+DDMM>>
N:	58
Object:	Poss. Radio G (SIMBAD class: RadioG = Radio Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=40+18 X-shaped and Z-shaped radio galaxy candidates (XRGs and ZRGs), in images from TGSS Alternative Data Release (TGSS ADR) images.
Ref:	=2022MNRAS.512.4308B
by	BHUKTA N. , PAL S., MONDAL S.K.
	Mon. Not. R. Astron. Soc., 512, 4308-4323 (2022)
	Search for X/Z-shaped radio sources from TGSS ADR 1.
o	Figs 7-8, Tables 1-2: <[BPM2022] JHHMM+DDMM> N=40+18.
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [BPN78]
[BPN78]	(Beckwith+Persson+Neugebauer+, 1978)
Write:	<<[BPN78] Pk N>>
N:	5
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=5 peaks of intensity of H2 lines in the Orion Nebula. See also [SUK94].
in source:	NAME Orion Nebula
Ref:	=1978ApJ...223..464B
by	BECKWITH S. , PERSSON S.E., NEUGEBAUER G., BECKLIN E.E.
	Astrophys. J., 223, 464-470 (1978)
	Observations of the molecular hydrogen emission from the Orion nebula.
o	Fig.2, Table 1: <[BPN78] Pk N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPR2007]
[BPR2007]	(Brassington+Ponman+Read, 2007)
Write:	<<[BPR2007] Mrk 266 A>> <<[BPR2007] Mrk 266 Diffuse N>> <<[BPR2007] Arp 222 NN>> <<[BPR2007] Arp 222 Diffuse>>
N:	2+3+15+1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra X-ray observations of interacting galaxies.
in source:	Mrk 266
in source:	APG 222
Ref:	=2007MNRAS.377.1439B
by	BRASSINGTON N.J. , PONMAN T.J., READ A.M.
	Mon. Not. R. Astron. Soc., 377, 1439-1456 (2007)
	The Chandra view of galaxy mergers.
o	Table 1, Fig.11: <[BPR2007] Mrk 266 A> (Nos A-B). Table 2, Fig.12: <[BPR2007] Mrk 266 Diffuse N> (Nos 1-3). Table 3, Fig.15: <[BPR2007] Arp 222 NN> (Nos 1-15), <[BPR2007] Arp 222 Diffuse> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPR2008]
[BPR2008]	(Berge+Pacaud+Refregier+, 2008)= (WL)
Write:	<<[BPR2008] WLNN>>
N:	7
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Joint Weak Lensing (WL in the format) and X-ray analysis from the CFHTLS and XMM-LSS surveys.
Ref:	=2008MNRAS.385..695B
by	BERGE J. , PACAUD F., REFREGIER A., MASSEY R., PIERRE M., AMARA A., BIRKINSHAW M., PAULIN-HENRIKSSON S., SMITH G.P., WILLIS J.
	Mon. Not. R. Astron. Soc., 385, 695-707 (2008)
	Combined analysis of weak lensing and X-ray blind surveys.
o	Table 1: <[BPR2008] WLNN> (Nos WL01-WL07).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPR2011]
[BPR2011]	(Belloche+Parise+Schuller+, 2011)
Write:	<<[BPR2011] Cha3-CNN>>
N:	29
Object:	Core (SIMBAD class: denseCore = Dense Core)
Note:	APEX Laboca 870µm observations of N=29 starless cores in Chameleon III.
in source:	NAME Cha III
Ref:	=2011A&A...535A...2B
by	BELLOCHE A. , PARISE B., SCHULLER F., ANDRE P., BONTEMPS S., MENTEN K.M.
	Astron. Astrophys., 535A, 2-2 (2011)
	Will the starless cores in Chamaeleon I and III turn prestellar?
o	Fig. 3, Tables 2-3: <[BPR2011] Cha3-CNN> (Nos C1-C29).
o	Paragraph 2.2 IRAS 13134-6264 is a probable misprint for IRAS 13134-6242. Footnote 9 MMS1 not in Simbad.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPR2016]
[BPR2016]	(Bina+Pello+Richard+, 2016)
Write:	<<[BPR2016] NNa>> <<[BPR2016] NNa(ext)>> <<[BPR2016] A1689 NNNN>> <<[BPR2016] A1689 LNNN>> <<[BPR2016] A1689 LNNa>>
N:	34
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	VLT MUSE spectroscopic observations of N=34 lensed images in the field of ACO 1689. See also [CBB2010b]. Use of archival HST ACS images.
in source:	ACO 1689
Ref:	=2016A&A...590A..14B
by	BINA D. , PELLO R., RICHARD J., LEWIS J., PATRICIO V., CANTALUPO S., HERENZ E.C., SOTO K., WEILBACHER P.M., BACON R., VERNET J.D.R., WISOTZKI L., CLEMENT B., CUBY J.G., LAGATTUTA D.J., SOUCAIL G., VERHAMME A.
	Astron. Astrophys., 590A, 14-14 (2016)
	MUSE observations of the lensing cluster Abell 1689.
o	Table 2, col(1): <[BPR2016] A1689 NNNN> N=12 among (Nos 518-1404), <[BPR2016] A1689 LNNN> N=16 among (Nos LN9-LN26), <[BPR2016] A1689 LNNa> N=6 among (Nos L1f-L50c). Table 2, col(2): <[BPR2016] NNa(ext)> N=34 among (Nos 51a-51b to 64).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPR98]
[BPR98]	(Bardelli+Pisani+Ramella+, 1998)
Write:	<<[BPR98] BNNNN>> <<[BPR98] TNNN>>
N:	16+21
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	Table 1: N=16 groups of galaxies in a Bidimensional sample (letter B in the format) in the ACO 3558 Complex Table 2: N=21 groups of galaxies in a Three-dimensional sample (letter T in the format) in the ACO 3558 Complex.
in source:	NAME ACO 3558 Complex:ACO 3558 = ACO 3558
in source:	ACO 3556
in source:	ACO 3562
in source:	SC 1327-31.0
in source:	SC 1329-31.0
Ref:	=1998MNRAS.300..589B
by	BARDELLI S. , PISANI A., RAMELLA M., ZUCCA E., ZAMORANI G.
	Mon. Not. R. Astron. Soc., 300, 589-598 (1998)
	A substructure analysis of the A3558 cluster complex.
o	Table 1: <[BPR98] BNNNN> N=16 among (Nos B109-B2240). Table 2: <[BPR98] TNNN> N=21 among (Nos T17-T599).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BPS
BPS	(Beers+Preston+Shectman)= (BS) = (CS) = (CTCS)
Write:	<<BPS BS FFFFF-NNNN>> <<BPS CS FFFFF-NNNN>>
Object:	* (SIMBAD class: Star)
Note:	In the format 'BS' stands for Burrell Schmidt telescope (hemisphere Nord), and 'CS' for Curtis Schmidt telescope (hemisphere South). The fields 'FFFFF' (always 5 digits fields) are those of the BS and CS telescopes, respectively at the Kitt Peak and Cerro Tololo observatories.
Ref:	=1982AJ.....87.1515P
by	PIER J.R.
	Astron. J., 87, 1515-1526 (1982)
	Stars of spectral types A and B in the southern galactic halo. I. UBV photometry.
o	<BPS CS FFFFF-NNN> N=234
Ref:	=1983ApJS...53..791P
by	PIER J.R.
	Astrophys. J., Suppl. Ser., 53, 791-813 (1983)
	AB stars in the southern galactic halo. II. Spectroscopy and radial velocities.
o	17 are new *, not in Paper I
o	<BPS CS FFFFF-NNN> N=224
Ref:	=1985AJ.....90.2089B
by	BEERS T.C. , PRESTON G.W., SHECTMAN S.A.
	Astron. J., 90, 2089-2102 (1985)
	A search for stars of very low metal abundance. I.
o	<BPS CS FFFFF-NNN> N=134
Ref:	=1988ApJS...67..461B
by	BEERS T.C. , PRESTON G.W., SHECTMAN S.A.
	Astrophys. J., Suppl. Ser., 67, 461-501 (1988)
	A catalog of candidate field horizontal-branch stars. I.
o	(Erratum) + erratum vol 70, 679
o	<BPS CS FFFFF-NNN> N=4408
Ref:	=1990PASP..102.1392D
by	DOINIDIS S.P. , BEERS T.C.
	Publ. Astron. Soc. Pac., 102, 1392-1399 (1990)
	Photoelectric UBV photometry of northern stars from the HK objective-prism survey.
o	<BPS BS FFFFF-NNN> N=139.
Ref:	=1991PASP..103..973D
by	DOINIDIS S.P. , BEERS T.C.
	Publ. Astron. Soc. Pac., 103, 973-986 (1991)
	Photoelectric UBV photometry of northern stars from the HK objective-prism survey. II.
o	(Erratum) 1992PASP..104..978D in table 4 for BS 16032
o	<BPS BS FFFFF-NNN> N=165
Ref:	=1991ApJS...76.1001P
by	PRESTON G.W. , SHECTMAN S.A., BEERS T.C.
	Astrophys. J., Suppl. Ser., 76, 1001-1031 (1991)
	Photoelectric UBV photometry of stars selected in the HK objective-prism survey.
o	Tables: <BPS CS FFFFF-NNNN> N=1782.
Ref:	=1992AJ....103..267B
by	BEERS T.C. , PRESTON G.W., SHECTMAN S.A., DOINIDIS S.P., GRIFFIN K.E.
	Astron. J., 103, 267-296 (1992)
	Spectroscopy of hot stars in the galactic halo.
o	<BPS CS FFFFF-NNN> N=769
Ref:	=1992AJ....103.1987B
by	BEERS T.C. , PRESTON G.W., SHECTMAN S.A.
	Astron. J., 103, 1987-2034 (1992)
	A search for stars of very low metal abundance. II.
o	<BPS CS FFFFF-NNN> N=1044
Ref:	=1994AJ....108..268B
by	BEERS T.C. , BESTMAN W., WILHELM R.
	Astron. J., 108, 268-270 (1994)
	Emission-line candidates from the northern HK survey.
o	Table 2: PC = PG, C = G.
o	<BPS BS FFFFF-NNN> N=158
Ref:	=1994AJ....108..538P
by	PRESTON G.W. , BEERS T.C., SHECTMAN S.A.
	Astron. J., 108, 538-554 (1994)
	The space density and kinematics of blue metal-poor main sequence stars near the solar circle.
o	<BPS CS FFFFF-NNN> N=175
Ref:	=1996AJ....112.1188B
by	BEERS T.C. , ROSSI S., ULRICH D., WILHELM R.
	Astron. J., 112, 1188-1196 (1996)
	Additional emission-line candidates from the HK survey.
o	Table 1: <BPS CS FFFFF-NNN> N=202. <BPS BS FFFFF-NNN> N=16
Ref:	=1996ApJS..103..433B
by	BEERS T.C. , WILHELM R., DOINIDIS S.P., MATTSON C.J.
	Astrophys. J., Suppl. Ser., 103, 433-466 (1996)
	A catalog of candidate field horizontal-branch and A-type stars. II.
o	Tables 3, 4: <BPS BS FFFFF-NNN> N=4175
Ref:	=1999AJ....117.2329W
by	WILHELM R. , BEERS T.C., SOMMER-LARSEN J., PIER J.R., LAYDEN A.C., FLYNN C., ROSSI S., CHRISTENSEN P.R.
	Astron. J., 117, 2329-2380 (1999)
	Spectroscopy of hot stars in the galactic halo. III. Analysis of a large sample of field horizontal-branch and other A-type stars.
o	Table 1: <BPS BS FFFFF-NNN> N=90, <BPS CS FFFFF-NNN> N=1031.
=E=	Catalogue in electronic form as J/PASP/102/1392
=E=	Catalogue in electronic form as J/PASP/103/973
=E=	Catalogue in electronic form as J/AJ/87/1515
=E=	Catalogue in electronic form as J/AJ/90/2089
=E=	Catalogue in electronic form as J/AJ/103/267
=E=	Catalogue in electronic form as J/AJ/103/1987
=E=	Catalogue in electronic form as J/AJ/108/268
=E=	Catalogue in electronic form as J/AJ/108/538
=E=	Catalogue in electronic form as J/AJ/112/1188
=E=	Catalogue in electronic form as J/ApJS/53/791
=E=	Catalogue in electronic form as J/ApJS/67/461
=E=	Catalogue in electronic form as J/ApJS/76/1001
=E=	Catalogue in electronic form as J/AJ/117/2329
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BPS
BPS	(Bappu+Parthasarathy+Scaria)
*****	Avoid the usage of BPS, prefer [BPS77]
Origin	of the Acronym: L (1983A&AS...51..277R)
Details on Acronym: [BPS2020]
[BPS2020]	(Berg +Pogge+Skillman+, 2020)
Write:	<<[BPS2020] NGC3184+xxx.x+yyy.y>>
N:	50
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	LBT MODS observations of N=52 HII regions in NGC 3184, as part of the CHemical Abundances Of Spirals (CHAOS) project. See also [BSC2015] for HII regions in NGC 628, [CPB2015] for HII regions in NGC 5194, [CPB2016] for HII regions in NGC 5457, and [RSP2021] for HII regions in NGC 2403.
in source:	NGC 3184
Ref:	=2020ApJ...893...96B
by	BERG D.A. , POGGE R.W., SKILLMAN E.D., CROXALL K.V., MOUSTAKAS J., ROGERS N.S.J., SUN J.
	Astrophys. J., 893, 96-96 (2020)
	CHAOS IV: gas-phase abundance trends from the first four CHAOS galaxies.
o	Table A1: <[BPS2020] NGC3184+xxx.x+yyy.y> N=50.
=E=	Catalogue in electronic form as <J/ApJ/893/96/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [BPS77]
[BPS77]	(Bappu+Parthasarathy+Scaria, 1977)= (BPS)
Write:	<<[BPS77] NNN>>
N:	298
Object:	Red * (SIMBAD class: Star)
in source:	Magellanic Clouds:LMC:30 Dor Nebula = 30 Dor Nebula
Ref:	=1977KodOB...2...85B
by	BAPPU M.K.V. , PARTHASARATHY M., SCARIA K.K.
	Kodaikanal Obs. Bull., 2, 85-88 (1977)
	A survey of red stars in the direction of the Large Magellanic Cloud.
o	Table 1: <[BPS77] NNN> (Nos 1-298).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPU2006]
[BPU2006]	(Bresolin+Pietrzynski+Urbaneja+, 2006)
Write:	<<[BPU2006] {A\|B} NN>>
N:	19+19
Object:	Supergiant * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 observations of blue supergiant stars in WLM.
in source:	DDO 221 = WLM Galaxy
Ref:	=2006ApJ...648.1007B
by	BRESOLIN F. , PIETRZYNSKI G., URBANEJA M.A., GIEREN W., KUDRITZKI R.-P., VENN K.A.
	Astrophys. J., 648, 1007-1019 (2006)
	The Araucaria project: VLT spectra of blue supergiants in WLM– classification and first abundances.
o	Table 1: <[BPU2006] A NN> (Nos 1-19), <[BPU2006] B NN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPV2008]
[BPV2008]	(Bassa+Pooley+Verbunt+, 2008)
Write:	<<[BPV2008] M 55 CXNN>> <<[BPV2008] NGC 6366 CXNNa>>
N:	31+14
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS observations of N=2 globular clusters.
in source:	M 55 = NGC 6809
in source:	NGC 6366
Ref:	=2008A&A...488..921B
by	BASSA C.G. , POOLEY D., VERBUNT F., HOMER L., ANDERSON S.F., LEWIN W.H.G.
	Astron. Astrophys., 488, 921-933 (2008)
	X-ray and optical observations of M55 and NGC6366: evidence for primordial binaries.
o	Table 2: <[BPV2008] M 55 CXNN> (Nos CX1-CX31). Table 3: <[BPV2008] NGC 6366 CXNNa> (Nos CX1a, CX1b, CX2-CX14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BPW2010]
[BPW2010]	(Bik+Puga+Waters+, 2010)
Write:	<<[BPW2010] NN>>
N:	29
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT SINFONI spectroscopy and Spitzer IRAC photometry of RCW 34.
in source:	RCW 34
Ref:	=2010ApJ...713..883B
by	BIK A. , PUGA E., WATERS L.B.F.M., HORROBIN M., HENNING Th., VASYUNINA T., BEUTHER H., LINZ H., KAPER L., VAN DEN ANCKER M., LENORZER A., CHURCHWELL E., KURTZ S., KOUWENHOVEN M.B.N., STOLTE A., DE KOTER A., THI W.F., COMERON F., WAELKENS C.
	Astrophys. J., 713, 883-899 (2010)
	Sequential star formation in RCW 34: a spectroscopic census of the stellar content of high-mass star-forming regions.
o	Fig. 10, Table 6: <[BPW2010] NN> (Nos 1-29).
o	Gum 29 is a misprint for Gum 19.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BQ
BQ	(Bright QSO)
*****	Avoid the usage of BQ, prefer FBQS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Br
Br	(Brun) (Not yet in Simbad)
*****	Avoid the usage of Br, prefer [B57]
Details on Acronym: Br
Br	(Brodskaja)
*****	Avoid the usage of Br, prefer [B53]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Br
Br	(Brodskaja)
*****	Avoid the usage of Br, prefer [B55b]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Br
Br	(Br)
*****	Avoid the usage of Br, prefer [BGR2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BR
BR	(B_j_,R survey)
Write:	<<BR BHHMM+DD>> <<BR BHHMM+DDMM>> <<BR BHHMM+DDMMe>> <<BR JHHMM+DDMM>>
Object:	QSO (SIMBAD class: QSO = Quasar)
Note:	QSOs from the APM multi-colour quasar survey (BR survey). Acronym BR is used when only the B and R UKST survey plates are used. Acronym BRI is used when all 3 i.e. B, R and I plates are used. 1994: 1st ref. with 'BR HHMM+DDMM' format 1996: 1st ref. with 'BR HHMM+DDMMe' format
Ref:	=1994ApJ...427L..13S
by	STORRIE-LOMBARDI L.J. , McMAHON R.G., IRWIN M.J., HAZARD C.
	Astrophys. J., 427, 13-16 (1994)
	Evolution of Lyman-limit absorption systems over the redshift range 0.40 < z < 4.69.
o	PKS 1354+1919 = PKS 1354+19, PKS 1424-1150 = PKS 1424-118
o	<BR HHMM+DDMM> N=7
Ref:	=1996ApJ...459L..53H
by	HU E.M. , McMAHON R.G., EGAMI E.
	Astrophys. J., 459, 53-56 (1996)
	Detection of a Ly α emission-line companion to the z=4.69 quasar BR 1202-0725.
o	<BR HHMM+DDMMe> (No. BR 1202-0725e).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Br
Br	(Brand+)
*****	Avoid the usage of Br, prefer Bran
Origin	of the Acronym: L (2000A&A...357..308G)
Details on Acronym: Br
Br	(Breysacher)
*****	Avoid the usage of Br, prefer Brey
Details on Acronym: [BR2001]
[BR2001]	(Bally+Reipurth, 2001)
Write:	<<[BR2001] HH NNN jet>> <<[BR2001] HH NNN W jet>> <<[BR2001] HH 502 N3 wing>> <<[BR2001] HH 504 bow>> <<[BR2001] HH NNN star>> <<[BR2001] HH 502 star A>> <<[BR2001] LLN>> <<[BR2001] HH CN>>
N:	11+13+3+1+7+3
Object:	Feature (SIMBAD class: Outflow_Candidate = Outflow Candidate)
Note:	Mayall 5m telescope MOSAIC narrow-band observations of the Orion Nebula. Study of HH jets. Format 'LLN' are LL Ori type bow shocks LL1 to LL7 in M 42 = Ori Nebula. Format 'HH CN' refers to candidate objects whose HH nature has not yet been firmly established (Nos C1-C3). See also [BOM2000], [BJJ2001b].
in source:	M 42 = NAME ORION NEBULA
in source:	NGC 1333
Ref:	=2001ApJ...546..299B
by	BALLY J. , REIPURTH B.
	Astrophys. J., 546, 299-323 (2001)
	Irradiated Herbig-Haro jets in the Orion nebula and near NGC 1333.
o	Table 2: <HH NNNWN> N=55, <HH NNNWWN> N=11. Table 2:<[BR2001] HH NNN jet> N=7, <[BR2001] HH NNN W jet> N=2, <[BR2001] HH 502 N3 wing> N=1, <[BR2001] HH 504 bow> N=1, <[BR2001] HH NNN star> N=13. Fig.2: <[BR2001] HH 502 star A> (Nos A-C). Table 5: <[BR2001] LLN> (Nos LL1 to LL7). Table 6: <[BR2001] HH CN> (Nos C1-C3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BR2009]
[BR2009]	(Brown+Rudnick, 2009)
Write:	<<[BR2009] J0809+39 W(Diff)>> <<[BR2009] J0809+39 FN>>
N:	2+7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	WSRT 351MHz and VLA 1.4GHz observations of the radio source [DR2006] J0809+39 and its components.
in source:	[DR2006] J0809+39
Ref:	=2009AJ....137.3158B
by	BROWN S. , RUDNICK L.
	Astron. J., 137, 3158-3171 (2009)
	Diffuse cluster-like radio emission in poor environments.
o	Fig. 1: Compact sources S1 and S2 are not in Simbad.
o	Fig.1: <[BR2009] J0809+39 W(Diff)> (Nos N(Diff), S(Diff)). Fig.2: <[BR2009] JHHMM+DD FN> (Nos F1-F7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BR2015]
[BR2015]	(Buckle+Richer, 2015)
Write:	<<[BR2015] NNN>>
N:	136
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	JCMT SCUBA-2 850µm and 450µm continuum observations of N=136 dust clumps in the field of the NGC 2264 molecular cloud.
in source:	NGC 2264
Ref:	=2015MNRAS.453.2006B
by	BUCKLE J.V. , RICHER J.S.
	Mon. Not. R. Astron. Soc., 453, 2006-2016 (2015)
	Wide-field SCUBA-2 observations of NGC 2264: submillimetre clumps and filaments.
o	Table A1: <[BR2015] NNN> (Nos 1-136).
=E=	Catalogue in electronic form as J/MNRAS/453/2006
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BR96]
[BR96]	(Belloni+Roser, 1996)
Write:	<<[BR96] Cl 0939+472 NNN>> <<[BR96] Cl 0016+161 NNN>>
N:	325+200
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	ClG 0939+4713 = ACO 851
in source:	ClG 0016+1609 = 1E 0015.9+1609
Ref:	=1996A&AS..118...65B
by	BELLONI P. , ROESER H.-J.
	Astron. Astrophys., Suppl. Ser., 118, 65-87 (1996)
	Galaxy population in distant galaxy clusters. I. Cl 0939+472 (z=0.41) and Cl0016+161 (z=0.54).
o	Table 4: <[BR96] Cl 0939+472 NNN> N=325 among (Nos 1-788). Table 5: <[BR96] Cl 0016+161 NNN> N=200 among (Nos 4-280).
=E=	Catalogue in electronic form as J/A+AS/118/65
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BRA2010]
[BRA2010]	(Brodwin+Ruel+Ade+, 2010)
Write:	<<[BRA2010] JHHMMSS.s+DDMMSS>>
N:	21
Object:	G (SIMBAD class: Galaxy)
Note:	Magellan Baade telescope IMACS optical spectroscopy of N=21 secure members of the massive galaxy cluster SPT-CL J0546-5345.
in source:	SPT-CL J0546-5345
Ref:	=2010ApJ...721...90B
by	BRODWIN M. , RUEL J., ADE P.A.R., AIRD K.A., ANDERSSON K., ASHBY M.L.N., BAUTZ M., BAZIN G., BENSON B.A., BLEEM L.E., CARLSTROM J.E., CHANG C.L., CRAWFORD T.M., CRITES A.T., DE HAAN T., DESAI S., DOBBS M.A., DUDLEY J.P., FAZIO G.G., FOLEY R.J., FORMAN W.R., GARMIRE G., GEORGE E.M., GLADDERS M.D., GONZALEZ A.H., HALVERSON N.W., HIGH F.W., HOLDER G.P., HOLZAPFEL W.L., HRUBES J.D., JONES C., JOY M., KEISLER R., KNOX L., LEE A.T., LEITCH E.M., LUEKER M., MARRONE D.P., McMAHON J.J., MEHL J., MEYER S.S., MOHR J.J., MONTROY T.E., MURRAY S.S., PADIN S., PLAGGE T., PRYKE C., REICHARDT C.L., REST A., RUHL J.E., SCHAFFER K.K., SHAW L., SHIROKOFF E., SONG J., SPIELER H.G., STALDER B., STANFORD S.A., STANISZEWSKI Z., STARK A.A., STUBBS C.W., VANDERLINDE K., VIEIRA J.D., VIKHLININ A., WILLIAMSON R., YANG Y., ZAHN O., ZENTENO A.
	Astrophys. J., 721, 90-97 (2010)
	SPT-CL J0546-5345: a massive z>1 galaxy cluster selected via the Sunyaev-Zel'dovich effect with the south pole telescope.
o	Fig. 1, Table 1: <[BRA2010] JHHMMSS.s+DDMMSS> N=21.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BRA2016]
[BRA2016]	(Borissova+Ramirez Alegria+Alonso+, 2016)
Write:	<<[BRA2016] CLNNN ObjN>> <<[BRA2016] DBSNNN ObjN>> <<[BRA2016] CLNNN ysocN>> <<[BRA2016] DBSNNN ysocNN>> <<[BRA2016] CLNNN Obj N>> (not recognised by Simbad, but found in literature) <<[BRA2016] DBSNNN Obj N>>
N:	10+11+22+26
Object:	* + Poss. YSO (SIMBAD class: Star)
Note:	ESO NTT SofI, VLT ISAAC, SOAR OSIRIS observations of N=21 stars and N=22 YSO candidates in four VVV young stellar cluster (CLNNN in the format, VVV), and of N=11 stars and N=26 YSO candidates in four additional young stellar clusters from the Dutra et al. 2003A&A...400..533D catalog (DBSNNN in the format, [DBS2003]).
in source:	VVV CL010
in source:	VVV CL012
in source:	VVV CL013
in source:	VVV CL059
in source:	[DBS2003] 75
in source:	[DBS2003] 93
in source:	[DBS2003] 100
in source:	[DBS2003] 130
Ref:	=2016AJ....152...74B
by	BORISSOVA J. , RAMIREZ ALEGRIA S., ALONSO J., LUCAS P.W., KURTEV R., MEDINA N., NAVARRO C., KUHN M., GROMADZKI M., RETAMALES G., FERNANDEZ M.A., AGURTO-GANGAS C., CHENE A.-N., MINNITI D., CONTRERAS PENA C., CATELAN M., DECANY I., THOMPSON M.A., MORALES E.F.E., AMIGO P.
	Astron. J., 152, 74-74 (2016)
	Young stellar clusters containing massive young stellar objects in the VVV survey.
o	Fig. 1, Table 2: <[BRA2016] CLNNN ObjN> N=10, <[BRA2016] DBSNNN ObjN> N=11. Table 4: <[BRA2016] CLNNN ysocN> N=22, <[BRA2016] DBSNNN ysocNN> N=26.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BRABCMS
BRABCMS	(van den Bergh+Racine+van Agt+Barnes+Coutts+Madore+Skill)
*****	Avoid the usage of BRABCMS, prefer VBRc
Details on Acronym: Braes
Braes	(Braes)
Write:	<<Braes NNNN>>
N:	1113
Object:	* (SIMBAD class: Star)
in source:	Ass Sco OB 1
Ref:	=1967BANS....2....1B
by	BRAES L.L.E.
	Bulletin of the Astronomical Institutes of the Netherlands, Supplement Series, 2, 1-58 (1967)
	Determination of proper motions in the region of the association Scorpius OBl.
o	misprint HD 152553 for 152353
o	Catalogue: <Braes NNNN> (Nos 1-1113)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Braid
Braid	(Braid+)
Write:	<<Braid NNN>>
N:	474
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Ref:	=1978MNRAS.182..241B
by	BRAID M.K. , MacGILLIVRAY H.T.
	Mon. Not. R. Astron. Soc., 182, 241-248 (1978)
	A finding list of southern clusters of galaxies -I.
o	<Braid NNN> (Nos 1-474)
Origin	of the Acronym: L (1987MNRAS.224..453C)
Details on Acronym: Bran
Bran	(Brand+)= (Br) = (BBW) = (BBWo)
Write:	<<BRAN NNNA>>
N:	526
Object:	Neb. Obj. (SIMBAD class: ISM = Interstellar Medium Object)
Stat:	is completely incorporated in Simbad
Ref:	=1986A&AS...65..537B
by	BRAND J. , BLITZ L., WOUTERLOOT J.G.A.
	Astron. Astrophys., Suppl. Ser., 65, 537-550 (1986)
	The velocity field of the outer Galaxy in the southern hemisphere. I. Catalogue of nebulous objects.
o	Table I: <Bran NNNA> (Nos 1-400), N=523
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BRB2003]
[BRB2003]	(Biggs+Rusin+Browne+, 2003)
Write:	<<[BRB2003] B0850+054 A>>
N:	2
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Stat:	is completely incorporated in Simbad
Note:	Images of the gravitational lens system CLASS B0850+054.
Ref:	=2003MNRAS.338.1084B
by	BIGGS A.D. , RUSIN D., BROWNE I.W.A., DE BRUYN A.G., JACKSON N.J., KOOPMANS L.V.E., McKEAN J.P., MYERS S.T., BLANDFORD R.D., CHAE K.-H., FASSNACHT C.D., NORBURY M.A., PEARSON T.J., PHILLIPS P.M., READHEAD A.C.S., WILKINSON P.N.
	Mon. Not. R. Astron. Soc., 338, 1084-1088 (2003)
	B0850+054: a new gravitational lens system from CLASS.
o	Text: <[BRB2003] B0850+054 A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BRB2005]
[BRB2005]	(Barrena+Ramella+Boschin+, 2005)= (VGCF)
Write:	<<[BRB2005] VNN>> <<[BRB2005] VN N>> <<[BRB2005] PNN NN>>
N:	48+9+9+10+3+2
Object:	Cluster of G + G in ClG (SIMBAD class: ClG = Cluster of Galaxies)
Note:	Development of the Voronoi Galaxy Cluster Finder (VGCF) technique by applying to galaxy catalogs. Comparison with PDCS cluster catalogue (PNN). 48 clusters are identified (Nos V1-V48). Member galaxies are identified in 5 VNN and 3 PNN clusters.
Ref:	=2005A&A...444..685B
by	BARRENA R. , RAMELLA M., BOSCHIN W., NONINO M., BIVIANO A., MEDIAVILLA E.
	Astron. Astrophys., 444, 685-695 (2005)
	VGCF detection of galaxy systems at intermediate redshifts.
o	In reference list: Postman, M., Lubin, L. M., Gunn, J.E., et al. (PLG96) should be 1996AJ....111..615P and not A&AS, 137, 83.
o	Table 5: <[BRB2005] VNN> (Nos V1-V48). Table 6: <[BRB2005] V4 N> (Nos 1-9), <[BRB2005] V6 N> (Nos 1-9), <[BRB2005] P33 NN> (Nos 1-10), <[BRB2005] P36 N> (Nos 1-3), <[BRB2005] P63 N> (Nos 1-2).
=E=	Catalogue in electronic form as J/A+A/444/685
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BRB98]
[BRB98]	(Bliton+Rizza+Burns+, 1998)
Write:	<<[BRB98] HHMM+DDdA>>
N:	23
Object:	Radio-G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC X-ray properties of a sample of 15 ACO clusters containing 23 NAT (Narrow-Angle Tailed) radio galaxies with a format 'HHMM+DDdA'
Ref:	=1998MNRAS.301..609B
by	BLITON M. , RIZZA E., BURNS J.O., OWEN F.N., LEDLOW M.J.
	Mon. Not. R. Astron. Soc., 301, 609-625 (1998)
	Cluster-subcluster mergers and the formation of narrow-angle tailed radio sources.
o	T.1, c(4): ROR is a internal ROSAT number not used in SIMBAD.
o	Table 1, col(2): <[BRB98] HHMM+DDdA> N=23.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BRC
BRC	(Bright Rimmed Cloud)
*****	Avoid the usage of BRC, prefer SFO
Origin	of the Acronym: L (1997ApJ...486L.141S)
Details on Acronym: [BRC2005]
[BRC2005]	(Baldacci+Rizzi+Clementini+, 2005)
Write:	<<[BRC2005] VNNN>>
N:	390 among 397
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	ESO VLT is used to identify variable stars in NGC 6822.
in source:	NGC 6822
Ref:	=2005A&A...431.1189B
by	BALDACCI L. , RIZZI L., CLEMENTINI G., HELD E.V.
	Astron. Astrophys., 431, 1189-1201 (2005)
	Variable stars in the dwarf irregular galaxy NGC6822: The photometric catalogue.
o	Table 2: <[BRC2005] VNNN> N=390 among (Nos V001-V397)
=E=	Catalogue in electronic form as J/A+A/431/1189
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BRC2010]
[BRC2010]	(Benaglia+Ribo+Combi+, 2010)
Write:	<<[BRC2010] N>>
N:	9
Object:	(NIR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Stat:	is completely incorporated in Simbad
Note:	ESO NTT JHKs photometry and spectroscopy of N=9 sources in the field of IRAS 16353-4636.
in source:	IRAS 16353-4636
Ref:	=2010A&A...523A..62B
by	BENAGLIA P. , RIBO M., COMBI J.A., ROMERO G.E., CHATY S., KORIBALSKI B., MIRABEL I.F., RODRIGUEZ L.F., BOSCH G.
	Astron. Astrophys., 523A, 62-62 (2010)
	Radio and IR study of the massive star-forming region IRAS 16353-4636.
o	Fig. 5, Table 3: <[BRC2010] N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BRC95]
[BRC95]	(Brewer+Richer+Crabtree, 1995)
Write:	<<[BRC95] C fF.NN>> <<[BRC95] M fF.NNNN>>
Object:	Late * (SIMBAD class: Star)
Note:	Table 7: candidate C stars, format 'C fF.NN', in 5 fields (f1-f5) Table 8: candidate M stars, format 'M fF.NNNN', in 5 fields (f1-f5) The 2 tables are presented in their complete form in the AAS CD-ROM See also [BRC96]
in source:	M 31 = NGC 224
Ref:	=1995AJ....109.2480B
by	BREWER J.P. , RICHER H.B., CRABTREE D.R.
	Astron. J., 109, 2480-2502 (1995)
	Late-type stars in M31. I. Photometric study of AGB stars and metallicity gradients.
o	Table 7: <[BRC95] C fF.NNNN>, Table 8: <[BRC95] M fF.NNNN>
=E=	Catalogue in electronic form as J/AJ/109/2480
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BRC96]
[BRC96]	(Brewer+Richer+Crabtree, 1996) (Not yet in Simbad)
Write:	<<[BRC96] F3-NN.N>> <<[BRC96] F4-NN.N>>
N:	87
Object:	Late * (SIMBAD class: Star)
Note:	See also [BRC96]
in source:	M 31 = NGC 224
Ref:	=1996AJ....112..491B
by	BREWER J.P. , RICHER H.B., CRABTREE D.R.
	Astron. J., 112, 491-508 (1996)
	Late-type stars in M31. II. C-, S-, and M-star spectra.
o	Table 1: C* '[BRC95] C fN.NNNN' not in Simbad
o	Table 1: <[BRC96] FN-NN.N> N=87
=E=	Catalogue in electronic form as J/AJ/112/491
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BRD2006]
[BRD2006]	(Bassino+Richtler+Dirsch, 2006)
Write:	<<[BRD2006] JHHMMSS.ss+DDMMSS.s>>
N:	136+104+126
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	Observations with the MOSAIC wide-field imager on CTIO 4m Blanco telescope. Photometric study of the globular cluster systems in 3 Fornax Cluster galaxies.
in source:	Fornax Cluster:NGC 1374 = NGC 1374
in source:	Fornax Cluster:NGC 1379 = NGC 1379
in source:	Fornax Cluster:NGC 1387 = NGC 1387
Ref:	=2006MNRAS.367..156B
by	BASSINO L.P. , RICHTLER T., DIRSCH B.
	Mon. Not. R. Astron. Soc., 367, 156-168 (2006)
	Globular cluster systems in low-luminosity early-type galaxies near the Fornax cluster centre.
o	Table 2: <[BRD2006] JHHMMSS.ss+DDMMSS.s> N=136+104+126.
=E=	Catalogue in electronic form as J/MNRAS/367/156
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Brey
Brey	(Breysacher)= (Br) = (Breys) = (Breysacher) = (JB)
Write:	<<Brey NNNa>>
N:	122
Object:	WR (SIMBAD class: WolfRayet* = Wolf-Rayet)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-100) in the 1st ref., and format 'NNNa' for new discovered WR stars inserted in RA. The first newly discovered was 'Brey 3a' (inserted between No. 3 and 4) in 1990A&A...236L..21H, then reclasified in 1991A&A...244L...9M.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1981A&AS...43..203B
by	BREYSACHER J.
	Astron. Astrophys., Suppl. Ser., 43, 203-207 (1981)
	Spectral classification of Wolf-Rayet stars in the Large Magellanic Cloud.
o	Table II: <Brey NNN> (Nos 1-100)
Ref:	=1990A&A...236L..21H
by	HEYDARI-MALAYERI M. , MELNICK J., VAN DROM E.
	Astron. Astrophys., 236, 21-None (1990)
	A peculiar high density HII blob ejected by a WC9 star in the Large Magellanic Cloud.
o	<Brey 3a> added
Ref:	=1991IAUS..143..513L
by	LORTET M.-C.
	IAU Symposium, held in Sanur, Bali, Indonesia, June 18-22, 1990. Ed. K.A. van der Hucht and B. Hidayat. "Wolf-Rayet stars and interrelations with other massive stars in galaxies", 143, 513-514 (1991)
	Nomenclature problems.
o	Table 1: <Brey NNa> N=15 'NNa', 14 are new.
Details on Acronym: Breys
Breys	(Breysacher)
*****	Avoid the usage of Breys, prefer Brey
Details on Acronym: Breysacher
Breysacher	(Breysacher)
*****	Avoid the usage of Breysacher, prefer Brey
Details on Acronym: [BRF2015]
[BRF2015]	(Bussmann+Riechers+Fialkov+, 2015)
Write:	<<[BRF2015] HELAISSNN.N>> <<[BRF2015] HXMMNN.N>> <<[BRF2015] HECDFSNN.N>> <<[BRF2015] HADFSNN.N>> <<[BRF2015] HCOSMOSNN.N>> <<[BRF2015] HELAISS02.Lens0>> <<[BRF2015] HXMMNN.LensN>> <<[BRF2015] HECDFSNN.LensN>> <<[BRF2015] HADFSNN.LensN>> <<[BRF2015] HCOSMOS01.Lens0>> <<[BRF2015] HELAISSNN SourceN>> (not recognised by Simbad, but found in literature) <<[BRF2015] HXMMNN SourceN>> <<[BRF2015] HECDFSNN SourceN>> <<[BRF2015] HADFSNN SourceN>> <<[BRF2015] HCOSMOSNN SourceN>>
N:	63+22
Object:	? + Grav. lens (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	ALMA 870µm observations of N=63 gravitationally lensed sources and N=22 gravitational lenses in the field of 29 HerMES dusty star-forming galaxies (DSFGs).
Ref:	=2015ApJ...812...43B
by	BUSSMANN R.S. , RIECHERS D., FIALKOV A., SCUDDER J., HAYWARD C.C., COWLEY W.I., BOCK J., CALANOG J., CHAPMAN S.C., COORAY A., DE BERNARDIS F., FARRAH D., FU H., GAVAZZI R., HOPWOOD R., IVISON R.J., JARVIS M., LACEY C., LOEB A., OLIVER S.J., PEREZ-FOURNON I., RIGOPOULOU D., ROSEBOOM I.G., SCOTT D., SMITH A.J., VIEIRA J.D., WANG L., WARDLOW J.
	Astrophys. J., 812, 43 (2015)
	HerMES: ALMA imaging of Herschel-selected dusty star-forming galaxies.
o	(Erratum) erratum vol. 815, art. 135 (2015)
o	Tables 1+3: <[BRF2015] HELAISSNN.N> N=4, <[BRF2015] HXMMNN.N> N=27, <[BRF2015] HECDFSNN.N> N=7, <[BRF2015] HADFSNN.N> N=19, <[BRF2015] HCOSMOSNN.N> N=6. Table 2: <[BRF2015] HELAISS02.Lens0> N=1, <[BRF2015] HXMMNN.LensN> N=13, <[BRF2015] HECDFSNN.LensN> N=2, <[BRF2015] HADFSNN.LensN> N=5, <[BRF2015] HCOSMOS01.Lens0> N=1.
=E=	Catalogue in electronic form as <J/ApJ/812/43/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BRF94]
[BRF94]	(Breen+Raychaudhury+Forman+, 1994)
Write:	<<[BRF94] SC 1327-312 HHMMSS.s+DDMMSS>> <<[BRF94] SC 1329-313 HHMMSS.s+DDMMSS>>
N:	4+7
Object:	G in ClG (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=4 galaxies in SC 1327-312 (each with a format HHMMSS.s+DDMMSS). N=7 galaxies in SC 1329-313 (each with a format HHMMSS.s+DDMMSS)
in source:	SC 1327-31.0
in source:	SC 1329-31.0
Ref:	=1994ApJ...424...59B
by	BREEN J. , RAYCHAUDHURY S., FORMAN W., JONES C.
	Astrophys. J., 424, 59-67 (1994)
	EINSTEIN X-ray observations of the core of the Shapley supercluster in northern Centaurus.
o	Table 1: <[BRF94] SC 1327-312 HHMMSS.s-DDMM SS> N=4. Table 1: <[BRF94] SC 1329-313 HHMMSS.s-DDMMSS> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Brh
Brh	(Bernhard+)= (Be)
Write:	<<Brh VNNN>>
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	2000IBVS.4920....1B: First ref. with Brh variables stars. Numbering is then continued with some objects till V138.
Ref:	=2000IBVS.4920....1B
by	BERNHARD K. , LLOYD C.
	IAU Inform. Bull. Var. Stars, 4920, 1-None (2000)
	New variables on the edge of the northern Milky Way - paper 1: BeV1-30.
o	<Brh VNN> (Nos V1-V30).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BRH2014]
[BRH2014]	(Bedin+Ruiz-Lapuente+Gonzalez Hernandez+, 2014)
Write:	<<[BRH2014] NNNN>>
N:	1148
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST ACS and WFC3 observations of N=1148 sources in the field of the remnant of SN 1572. See also [RCM2004].
Ref:	=2014MNRAS.439..354B
by	BEDIN L.R. , RUIZ-LAPUENTE P., GONZALEZ HERNANDEZ J.I., CANAL R., FILIPPENKO A.V., MENDEZ J.
	Mon. Not. R. Astron. Soc., 439, 354-371 (2014)
	Improved Hubble Space Telescope proper motions for Tycho-G and other stars in the remnant of Tycho's Supernova 1572.
o	Table 2: <[BRH2014] NNNN> (Nos 1-1148). Fig. 13, Tables 2-3: <[RCM2004] Tycho AN> (Nos W-Z, A2, C3, P1-P2) added, <[RCM2004] Tycho AAN> (Nos AA-AC, AD1-AD2, AE-AH, AI1-AI2, AJ-AN).
=E=	Catalogue in electronic form as <J/MNRAS/439/354/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BRHT
BRHT	(Bhatia+Read+Hatzidimitriou+Tritton)
Write:	<<BRHT NNa>>
N:	64x2
Object:	Binary OCl (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	N=64 close pairs of star clusters, each cluster in the pair being named 'NNa' and 'NNb'
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1991A&AS...87..335B
by	BHATIA R.K. , READ M.A., HATZIDIMITRIOU D., TRITTON S.
	Astron. Astrophys., Suppl. Ser., 87, 335-352 (1991)
	A catalogue of binary star cluster candidates in the Large Magellanic Cloud.
o	Table 1: <BRHT NNa> (Nos 1a-64a, 1b-64b)
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: BRI
BRI	(B_j_,R,I survey)
Write:	<<BRI BHHMM+DD>> <<BRI BHHMM+DDMM>> <<BRI JHHMM+DDMM>>
Object:	QSO (SIMBAD class: QSO = Quasar)
Note:	QSOs from the APM multi-colour quasar survey (BRI survey). Acronym BRI is used when all 3 i.e. B, R and I UKST survey plates are used. Acronym BR is used when only the B and R plates are used. 1990: 1st reference from this survey, with the format HHMM+DD. In this ref., N=10. 1991: 1st reference from this survey, with the format HHMM+DDMM. In this ref., N=1. 2001: The authors have in preparation objects 'BRI' with 2 formats BHHMM+DDMM and JHHMM+DDMM.
Ref:	=1990Gemin..30....6I
by	IRWIN M. , McMAHON R.
	GEMINI Newsletter Royal Greenwich Obs., 30, 6-None (1990)
	Yet more z>4 QSOs discovered using the INT.
o	<BRI HHMM+DD> N=10
Ref:	=1991MNRAS.252p..61I
by	IRWIN M. , McMAHON R.G., REID N.
	Mon. Not. R. Astron. Soc., 252, part no 16, 61-64 (1991)
	A star of exceedingly low luminosity.
o	<BRI HHMM+DDMM> N=1: BRI 0021-0214
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Briceno
Briceno	(Briceno+)
*****	Avoid the usage of Briceno, prefer [BCG93]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BRJ2015]
[BRJ2015]	(Beuther+Ragan+Johnston+, 2015)
Write:	<<[BRJ2015] NN>>
N:	12
Object:	Core (SIMBAD class: denseCore = Dense Core)
Note:	PdBI 3.2mm continuum observations of N=12 cores in the high-mass star-forming filament IRDC 18223.
in source:	NAME IRDC 18223-3
Ref:	=2015A&A...584A..67B
by	BEUTHER H. , RAGAN S.E., JOHNSTON K., HENNING Th., HACAR A., KAINULAINEN J.T.
	Astron. Astrophys., 584A, 67-67 (2015)
	Filament fragmentation in high-mass star formation.
o	Table 1: <[BRJ2015] NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BRK2009]
[BRK2009]	(Bresolin+Ryan-Weber+Kennicutt+, 2009)
Write:	<<[BRK2009] NN>> <<[BRK2009] Background G N>>
N:	49+9
Object:	HII + EmG (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 spectroscopy of HII regions in the outer disk of M83.
in source:	M 83 = NGC 5236
Ref:	=2009ApJ...695..580B
by	BRESOLIN F. , RYAN-WEBER E., KENNICUTT R.C., GODDARD Q.
	Astrophys. J., 695, 580-595 (2009)
	The flat oxygen abundance gradient in the extended disk of M83.
o	Tables 1-2: <[BRK2009] NN> (Nos 1-49). Table 4: <[BRK2009] Background G N> (Nos 1-9).
=E=	Catalogue in electronic form as <J/ApJ/695/580/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BRLT
BRLT	(?)
Write:	<<BRLT NNN>>
N:	68
Object:	Brown Dwarf (SIMBAD class: BrownD* = Brown Dwarf)
Note:	VLT X-shooter spectroscopy of N=68 L and T dwarfs from the UKIDSS LAS DR7 (ULAS).
Ref:	=2013MNRAS.430.1171D
by	DAY-JONES A.C. , MAROCCO F., PINFIELD D.J., ZHANG Z.H., BURNINGHAM B., DEACON N., RUIZ M.T., GALLARDO J., JONES H.R.A., LUCAS P.W.L., JENKINS J.S., GOMES J., FOLKES S.L., CLARKE J.R.A.
	Mon. Not. R. Astron. Soc., 430, 1171-1187 (2013)
	The sub-stellar birth rate from UKIDSS.
o	Table 1: <BRLT NNN> N=68 among (Nos 1-344).
=E=	Catalogue in electronic form as <J/MNRAS/430/1171/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BRN2015]
[BRN2015]	(Barba+Roman-Lopes+Nilo Castellon+, 2015)= (La Serena)
Write:	<<[BRN2015] La Serena NNN>>
N:	493
Object:	Poss. Cluster of * (SIMBAD class: Cluster*_Candidate = Cluster of Stars Candidate)
Note:	Search for infrared star cluster candidates in the ESO Public Survey "VISTA Variables in the Via Lactea".
Ref:	=2015A&A...581A.120B
by	BARBA R.H. , ROMAN-LOPES A., NILO CASTELLON J.L., FIRPO V., MINNITI D., LUCAS P., EMERSON J.P., HEMPEL M., SOTO M., SAITO R.K.
	Astron. Astrophys., 581A, 120-120 (2015)
	Hundreds of new cluster candidates in the VISTA Variables in the Via Lactea survey DR1.
o	Table 1: <[BRN2015] La Serena NNN> (Nos 1-493).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Bro
Bro	(Brorfelde telescope)
Write:	<<Bro YY-N>>
N:	3
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Ref:	=1994A&A...291L..17P
by	PEDERSEN H.
	Astron. Astrophys., 291, 17-18 (1994)
	Optical studies of the field of GRB 940301.
o	<Bro YY-N> N=3
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Bro05
Bro05	(Brodie+, 2005)
*****	Avoid the usage of Bro05, prefer [BSD2005]
Origin	of the Acronym: L (2005A&A...443..413L)
Details on Acronym: Brodskaja
Brodskaja	(Brodskaja)
*****	Avoid the usage of Brodskaja, prefer [B53]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Brodskaja
Brodskaja	(Brodskaja)
*****	Avoid the usage of Brodskaja, prefer [B55b]
Origin	of the Acronym: L (1959ApJ...130...69B)
Details on Acronym: Brodskaya
Brodskaya	(Brodskaja)
*****	Avoid the usage of Brodskaya, prefer [B53]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Brodskaya
Brodskaya	(Brodskaja)
*****	Avoid the usage of Brodskaya, prefer [B55b]
Origin	of the Acronym: L (1959ApJ...130...69B)
Details on Acronym: BROS
BROS	(Blazar Radio and Optical Survey) (Not yet in Simbad)
Write:	<<BROS JHHMM.m+DDMM>>
N:	88211
Object:	Poss. Blazar (SIMBAD class: Blazar_Candidate = Blazar Candidate)
Note:	N=88211 blazar candidates selected from the TGSS-NVSS catalog (De Gasperin et al., 2018MNRAS.474.5008D), located at decl.>-40° and outside the galactic plane (∣b∣>10°).
Ref:	=2020ApJ...901....3I
by	ITOH R. , UTSUMI Y., INOUE Y., OHTA K., DOI A., MOROKUMA T., KAWABATA K.S., TANAKA Y.T.
	Astrophys. J., 901, 3-3 (2020)
	Blazar Radio and Optical Survey (BROS): a catalog of blazar candidates showing flat radio spectrum and their optical identification in Pan-STARRS1 surveys.
o	<BROS JHHMM.m+DDMM> N=88211.
=E=	Catalogue in electronic form as <J/ApJ/901/3/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BRP2005]
[BRP2005]	(Brassington+Read+Ponman, 2005)
Write:	<<[BRP2005] HN>> <<[BRP2005] NN>>
N:	4+16
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of Arp 270: N=16 X-ray point sources are detected, and compared with ROSAT HRI sources 'HN'.
in source:	APG 270
Ref:	=2005MNRAS.360..801B
by	BRASSINGTON N.J. , READ A.M., PONMAN T.J.
	Mon. Not. R. Astron. Soc., 360, 801-815 (2005)
	Chandra observations of the interacting galaxies NGC 3395/3396 (Arp 270).
o	Fig.1, Table 1: <[BRP2005] HN> (Nos H1-H4). Fig.4, Table 2: <[BRP2005] NN> (Nos 1-16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BRP2016]
[BRP2016]	(Beasley+Romanowsky+Pota+, 2016)
Write:	<<[BRP2016] GCNN>> <<[BRP2016] N17>> <<[BRP2016] StarN>>
N:	6+1+3
Object:	GlCl + * + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	GTC OSIRIS spectroscopic observations of VCC 1287. Use of archival CFHT MegaCam images.
in source:	VCC 1287
Ref:	=2016ApJ...819L..20B
by	BEASLEY M.A. , ROMANOWSKY A.J., POTA V., MARTIN-NAVARRO I., MARTINEZ DELGADO D., NEYER F., DEICH A.L.
	Astrophys. J., 819L, 20 (2016)
	An overmassive dark halo around an ultra-diffuse galaxy in the Virgo cluster.
o	Table 1: <[BRP2016] GCNN> N=6 among (Nos GC10 to GC21), <[BRP2016] N17> N=1, <[BRP2016] StarN> (Nos Star1-Star3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BRR2002]
[BRR2002]	(Braje+Romani+Roberts+, 2002)
Write:	<<[BRR2002] NN>>
N:	21
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of GeV J1809-2327, identified with [BRR2002] 5.
in source:	GeV J1809-2327
Ref:	=2002ApJ...565L..91B
by	BRAJE T.M. , ROMANI R.W., ROBERTS M.S.E., KAWAI N.
	Astrophys. J., 565, 91-95 (2002)
	Chandra imaging of the γ-ray source GeV J1809-2327.
o	Table 1: <[BRR2002] NN> (Nos 1-21).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BRR2009]
[BRR2009]	(Bai+Rieke+Rieke+, 2009)
Write:	<<[BRR2009] DD.ddddd+DD.ddddd>>
N:	109
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Spitzer MIPS observations of the cluster A3266.
in source:	ACO 3266
Ref:	=2009ApJ...693.1840B
by	BAI L. , RIEKE G.H., RIEKE M.J., CHRISTLEIN D., ZABLUDOFF A.I.
	Astrophys. J., 693, 1840-1850 (2009)
	The infrared luminosity functions of rich clusters.
o	Table 1: <[BRR2009] DD.ddddd+DD.ddddd> N=109.
=E=	Catalogue in electronic form as <J/ApJ/693/1840/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BRRG
BRRG	(Barba+Rubio+Roth+Garcia)
Write:	<<BRRG NNN>> <<BRRG {A\|B\|I\|P\|S}N>>
N:	184+3+1+4+1+3
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	IR images of the region LHA 120-N 11B in the LMC, combined with HST WFPC2 archives. N=184 IR sources in the field of LHA 120-N 11B. N=3 nebular arcs (Nos A1-A3), N=4 finger-like features (Nos P1-P4), N=1 sphere around PGMW 3040, N=1 filamentary structure (No. S1), N=3 PDRs (PhotoDissociation Regions) (Nos I1-I3).
in source:	Magellanic Clouds:LMC:LHA 120-N 11B = LHA 120-N 11B
Ref:	=2003AJ....125.1940B
by	BARBA R.H. , RUBIO M., ROTH M.R., GARCIA J.
	Astron. J., 125, 1940-1957 (2003)
	Active star formation in the N11B nebula in the Large Magellanic Cloud: a sequential star formation scenario confirmed.
o	CH3OH Maser = [EWN94] 045640.87-662905.0.
o	Table 1: <BRRG NNN> (Nos 1-184). Fig.8: <BRRG AN> (Nos A1-A3, P1-P4, B1, S1). Fig.10: <BRRG AN> (Nos I1-I3).
=E=	Catalogue in electronic form as J/AJ/125/1940
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BRS2007]
[BRS2007]	(Becker+Rauch+Sargent, 2007) (Not yet in Simbad)
Write:	<<[BRS2007] QSO JHHMM+DDMM abs N.NNN>>
N:	88
Object:	Absorber
Note:	HIRES spectrograph on Keck I observations.
Ref:	=2007ApJ...662...72B
by	BECKER G.D. , RAUCH M., SARGENT W.L.W.
	Astrophys. J., 662, 72-93 (2007)
	The evolution of optical depth in the Lyα forest: evidence against reionization at z~6.
o	Table 1: <[BRS2007] QSO JHHMM+DDMM abs N.NNN> N=88.
=E=	Catalogue in electronic form as J/ApJ/662/72
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BRS2011]
[BRS2011]	(Brodie+Romanowky+Strader+, 2011)
Write:	<<[BRS2011] B1>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	CFHT Megacam observations of N=1 background galaxy in the field of M87.
in source:	NAME Virgo Cluster
Ref:	=2011AJ....142..199B
by	BRODIE J.P. , ROMANOWSKY A.J., STRADER J., FORBES D.A.
	Astron. J., 142, 199 (2011)
	The relationships among compact stellar systems: a fresh view of ultracompact dwarfs.
o	Table 1: <[BRS2011] B1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BRS2016]
[BRS2016]	(Bayliss+Ruel+Stubbs+, 2016)
Write:	<<[BRS2016] JHHMMSS.ss+DDMMSS.s>> <<[BRS2016] SPT-CL JHHMM+DDMM A.N>>
N:	2243+12
Object:	Grav. lensed image + G (SIMBAD class: Unknown = Object of Unknown Nature)
Notes:	Gemini South GMOS spectroscopic observations of N=2243 galaxies in N=62 galaxy clusters detected in the 2500 deg² SPT-SZ survey. N=12 images lensed by N=8 cluster of galaxies. See also [RBB2014].
Ref:	=2016ApJS..227....3B
by	BAYLISS M.B. , RUEL J., STUBBS C.W., ALLEN S.W., APPLEGATE D.E., ASHBY M.L.N., BAUTZ M., BENSON B.A., BLEEM L.E., BOCQUET S., BRODWIN M., CAPASSO R., CARLSTROM J.E., CHANG C.L., CHIU I., CHO H.-M., CLOCCHIATTI A., CRAWFORD T.M., CRITES A.T., DE HAAN T., DESAI S., DIETRICH J.P., DOBBS M.A., DOUCOULIAGOS A.N., FOLEY R.J., FORMAN W.R., GARMIRE G.P., GEORGE E.M., GLADDERS M.D., GONZALEZ A.H., GUPTA N., HALVERSON N.W., HLAVACEK-LARRONDO J., HOEKSTRA H., HOLDER G.P., HOLZAPFEL W.L., HOU Z., HRUBES J.D., HUANG N., JONES C., KEISLER R., KNOX L., LEE A.T., LEITCH E.M., VON DER LINDEN A., LUONG-VAN D., MANTZ A., MARRONE D.P., McDONALD M., McMAHON J.J., MEYER S.S., MOCANU L.M., MOHR J.J., MURRAY S.S., PADIN S., PRYKE C., RAPETTI D., REICHARDT C.L., REST A., RUHL J.E., SALIWANCHIK B.R., SARO A., SAYRE J.T., SCHAFFER K.K., SCHRABBACK T., SHIROKOFF E., SONG J., SPIELER H.G., STALDER B., STANFORD S.A., STANISZEWSKI Z., STARK A.A., STORY K.T., VANDERLINDE K., VIEIRA J.D., VIKHLININ A., WILLIAMSON R., ZENTENO A.
	Astrophys. J., Suppl. Ser., 227, 3-3 (2016)
	SPT-GMOS: a Gemini/GMOS-South spectroscopic survey of galaxy clusters in the SPT-SZ survey.
o	Table 3: <[BRS2016] JHHMMSS.ss+DDMMSS.s> N=2243. Table 4: <[BRS2016] SPT-CL JHHMM+DDMM A.N> N=12.
=E=	Catalogue in electronic form as J/ApJS/227/3
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BRS93]
[BRS93]	(Barbieri+Rafanelli+Schulz+, 1993)
Write:	<<[BRS93] A>> <<[BRS93] AN>>
N:	5+5
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST FOC observations of NGC 6240
in source:	NGC 6240
Ref:	=1993A&A...273....1B
by	BARBIERI C. , RAFANELLI P., SCHULZ H., ALBRECHT R., BLADES J.C., BOKSENBERG A., CRANE P., DEHARVENG J.M., DISNEY M.J., JAKOBSEN P., KAMPERMAN T.M., KING I.R., MACCHETTO F., MacKAY C.D., PARESCE F., WEIGELT G., BAXTER D., GREENFIELD P., JEDRZEWSKI R., NOTA A., SPARKS W.B.
	Astron. Astrophys., 273, 1-5 (1993)
	Compact subarcsec structures of the double nucleus of NGC 6240 revealed with HST.
o	Figs 2a, 2b: <[BRS93] A> (Nos A-E), <[BRS93] AN> (Nos A1-A3, B1)
Ref:	=1997A&A...327..901R
by	RAFANELLI P. , SCHULZ H., BARBIERI C., KOMOSSA S., MEBOLD U., BARUFFOLO A., RADOVICH M.
	Astron. Astrophys., 327, 901-908 (1997)
	Subarcsec structures in the double nucleus of NGC 6240 disclosed with HST at 370, 430 and 500nm.
o	Table 1: <[BRS93] AN> No. A4 added
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BRT2016]
[BRT2016]	(Burenin+Revnivtsev+Tkachenko+, 2016)= (400d)
Write:	<<[BRT2016] 400d JHHMMSS.s+DDMMSS>>
N:	8
Object:	Catacl. V* (SIMBAD class: CataclyV* = Cataclysmic Binary)
Note:	Russian-Turkish 1.5-m telescope (RTT-150), Special Astrophysical Observatory 6-m BTA telescope, Sayan Observatory 1.6-m AZT-33IK telescope observations of N=8 cataclysmic variables (CVs) identified among the X-ray sources from the 400 sq. deg. X-ray survey based on ROSAT pointing data (400d). See also [TRB2015]. Use of SDSS DR12 data.
Ref:	=2016AstL...42..240B
by	BURENIN R.A. , REVNIVTSEV M.G., TKACHENKO A.Y., VOROB'EV V.S., SEMENA A.N., MESHCHERYAKOV A.V., DODONOV S.N., ESELEVICH M.V., PAVLINSKY M.N.
	AstL, 42, 240-250 (2016)
	Sample of cataclysmic variables detected in the 400d X-ray survey.
o	Table 1: <[BRT2016] 400d JHHMMSS.s+DDMMSS> N=8.
o	2016PAZh...42..273B
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Bru
Bru	(Brunet+)
*****	Avoid the usage of Bru, prefer BI
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Bruck
Bruck	(Bruck)= (B) = (E)
Write:	<<Bruck NNN>>
N:	168
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Charts
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1976ORROE...1....1B
by	BRUCK M.T.
	Occasional Reports R. Obs., 1, 1-None (1976)
	Star clusters in the Small Magellanic Cloud.
o	<Bruck NNN> N=168
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: Brun
Brun	(Brun) (Not yet in Simbad)
*****	Avoid the usage of Brun, prefer [B57]
Details on Acronym: Brun
Brun	(Brun)
Write:	<<Brun NNNN>>
N:	about 1200
Object:	* in Cluster (SIMBAD class: Star)
in source:	NAME Orion Nebula
Ref:	=1935POLyo...1...12B
by	BRUN A.
	Publ. Obs. de Lyon, 1, 12-None (1935)
	La nebuleuse d'Orion et ses etoiles variables.
o	<Brun NNNN>
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BRW2009]
[BRW2009]	(Ben Bekhti+Richter+Winkel+, 2009)
Write:	<<[BRW2009] JHHMMSS+DDMMSS>>
N:	26
Object:	HI Clump (SIMBAD class: HI = HI (21cm) Source)
Note:	WSRT and VLA HI observations of clumps along four lines of sight through the Galactic halo.
Ref:	=2009A&A...503..483B
by	BEN BEKHTI N. , RICHTER P., WINKEL B., KENN F., WESTMEIER T.
	Astron. Astrophys., 503, 483-493 (2009)
	High-resolution 21-cm observations of low-column density gas clumps in the Milky way halo.
o	Table 3: <[BRW2009] JHHMMSS+DDMMSS> N=26.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BRY2005]
[BRY2005]	(Bower+Roberts+Yusef-Zadeh+, 2005)
Write:	<<[BRY2005] JHHMMSS.sss+DDMMSS.sss>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Discovery of a transient radio source 0.1 pc from Sgr A*, resolved into two components. VLA observations. The transient, CXOGC J174540.0-290031, was also detected in X-ray by Chandra and XMM-Newton (2005ApJ...633..228M and 2005A&A...443..571P).
Ref:	=2005ApJ...633..218B
by	BOWER G.C. , ROBERTS D.A., YUSEF-ZADEH F., BACKER D.C., COTTON W.D., GOSS W.M., LANG C.C., LITHWICK Y.
	Astrophys. J., 633, 218-227 (2005)
	A radio transient 0.1 parsecs from Sagittarius A.*
o	Porquet et al, astroph, published in 2005A&A...443..571P
o	Text: <[BRY2005] JHHMMSS.sss+DDMMSS.sss> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Bs
Bs	(Bernes)
*****	Avoid the usage of Bs, prefer [B77]
Details on Acronym: BS
BS	(Burell Schmidt telescope)
*****	Avoid the usage of BS, prefer BPS
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BS
BS	(Baade+Swope)
*****	Avoid the usage of BS, prefer [BS61]
Origin	of the Acronym: L (2004AJ....127..861B)
Details on Acronym: BS
BS	(Bohm+Solf)
*****	Avoid the usage of BS, prefer [BS94]
Origin	of the Acronym: L (1995A&A...296..431R)
Details on Acronym: BS
BS	(Bica+Schmitt)
*****	Avoid the usage of BS, prefer [BS95]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BS
BS	(Bahcall+Soneira)
*****	Avoid the usage of BS, prefer BSCG
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BS
BS	(Bright * catalog)
====>	Equivalent to: HR
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BS
BS	(B. Stenholm)
*****	Avoid the usage of BS, prefer [S75]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BS2000]
[BS2000]	(Beasley+Sharples, 2000)
Write:	<<[BS2000] NGC 253 NN>> <<[BS2000] NGC 55 NN>>
N:	91+84
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Stat:	is completely incorporated in Simbad
Note:	In NGC 253: N=91 globular cluster candidates (Nos 1-91). In NGC 55: N=84 globular cluster candidates (Nos 1-84) and See also [B86c] and [LA83].
in source:	NGC 253
in source:	NGC 55
Ref:	=2000MNRAS.311..673B
by	BEASLEY M.A. , SHARPLES R.M.
	Mon. Not. R. Astron. Soc., 311, 673-682 (2000)
	Spectroscopy of globular cluster candidates in the Sculptor group galaxies NGC 253 and 55.
o	Tables 2, 3: numbering in column (1) not used, objects are designated [LA83] or [B86c] in SIMBAD. In ref list ALCAINO 1984AJ.....89..814A instead of ApJ.89.6, BLECHA 1986A&A...154..321B instead of A&A.154.32
o	Table 6: <[BS2000] NGC 253 NN> (Nos 1-91), <[BS2000] NGC 55 NN> (Nos 1-84).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BS2002]
[BS2002]	(Brady+Schwartz, 2002)
Write:	<<[BS2002] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host G of SN 2002KF.
Ref:	=2002IAUC.8040....1B
by	BRADY S. , SCHWARTZ M.
	IAU Circ., 8040, 1-None (2002)
	Supernova 2002kf.
o	<[BS2002] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BS2003]
[BS2003]	(Bonanos+Stanek, 2003)
Write:	<<[BS2003] JHHMMSS.s+DDMMSS.s>>
N:	112
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS1 archival observations of M 83. Search for Cepheids. See also [TTS2003].
in source:	M 83 = NGC 5236
Ref:	=2003ApJ...591L.111B
by	BONANOS A.Z. , STANEK K.Z.
	Astrophys. J., 591, 111-114 (2003)
	Reanalysis of Very Large Telescope data for M83 with image subtraction–Ninefold increase in number of Cepheids.
o	Table 1: <[BS2003] JHHMMSS.s+DDMMSS.s> N=112. Fig.4: <[BS2003] JHHMMSS.s+DDMMSS.s> N=12.
=E=	Catalogue in electronic form as J/ApJ/591/L111
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BS2011]
[BS2011]	(Bower+Saul, 2011)
Write:	<<[BS2011] JHHMMSS.s+DDMMSS.s>>
N:	10
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 1.4GHz multi-epoch observations of the field of 3C 286.
in source:	3C 286
Ref:	=2011ApJ...728L..14B
by	BOWER G.C. , SAUL D.
	Astrophys. J., 728L, 14 (2011)
	A search for radio transients in very large array archival images of the 3C 286 field.
o	Table 1: <[BS2011] JHHMMSS.s+DDMMSS.s> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BS2011b]
[BS2011b]	(Bayliss+Sackett, 2011)
Write:	<<[BS2011b] SL-N>>
N:	6
Object:	EB+EB?+EP (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Search for transiting hot Jupiter planets in the SuperLupus Survey.
Ref:	=2011ApJ...743..103B
by	BAYLISS D.D.R. , SACKETT P.D.
	Astrophys. J., 743, 103 (2011)
	The frequency of hot jupiters in the galaxy: results from the SuperLupus survey.
o	Table 2: <[BS2011b] SL-N> N=6 among (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BS2017]
[BS2017]	(Bravo-Guerrero+Stevens, 2017)
Write:	<<[BS2017] NN>>
N:	45
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS observations of N=45 point sources in the field of NGC 2782.
in source:	NGC 2782
Ref:	=2017MNRAS.467.3788B
by	BRAVO-GUERRERO J. , STEVENS I.R.
	Mon. Not. R. Astron. Soc., 467, 3788-3800 (2017)
	Superwind evolution: the young starburst-driven wind galaxy NGC 2782.
o	Fig. 5, Table 1: <[BS2017] NN> (Nos 1-45).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BS61]
[BS61]	(Baade+Swope, 1961)= (BS) = (Draco)
Write:	<<[BS61] A>> <<[BS61] AN>> <<[BS61] ggg>> <<[BS61] NNNa>>
N:	25+4+3+595+3
Object:	* (SIMBAD class: Star)
Note:	Table II: Standard stars, (Nos A-Z) No. I missing, (Nos C1-C2, Q1-Q2), and (Nos alf, bet, gam). Table C: stars in Draco Dwarf Galaxy (Nos NNN, NNNa). See also BASV for V*.
in source:	NAME Draco Dwarf Galaxy
Ref:	=1961AJ.....66..300B
by	BAADE W. , SWOPE H.H.
	Astron. J., 66, 300-347 (1961)
	The Draco system, a dwarf galaxy.
o	Tables IV, V, VI, A, B, Plate III: <BASV NNN> (Nos 1-203). Table II: <[BS61] A> (Nos A-Z, No. I missing), <[BS61] AN> (Nos C1-C2, Q1-Q2), <[BS61] aaa> (Nos alf, bet, gam). Table C, Plate IV: <[BS61] NNNa> (Nos 1-595, 161a, 162a, 357a).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BS63]
[BS63]	(Baade+Swope, 1963)
Write:	<<[BS63] A>> <<[BS63] VNN>> <<[BS63] ANNNa>> <<[BS63] BNNNa>>
N:	23+54+545
Object:	* (SIMBAD class: Star)
Note:	Finding charts. Table I: sequence stars, N=23 among (Nos A-Z). Table III: N=54 V* among (Nos V1-V60), field IV in M 31. Table D: N=546 stars among (Nos A1-A307 and B1-B284), field IV in M 31 Fields I and III in M 31: see BASW, Field II in M 31: see Gapo.
in source:	M 31 = NGC 224
Ref:	=1963AJ.....68..435B
by	BAADE W. , SWOPE H.H.
	Astron. J., 68, 435-470 (1963)
	Variable star field 96' south preceeding the nucleous of the Andromeda galaxy.
o	Table I: <[BS63] A> N=23 among (Nos A-Z). Table III: <[BS63] VNN> N=54 among (Nos 1-60). Table D: <[BS63] ANNNa> N=546 among (Nos A1-A307, B1-B284, B60a, B60b, B68a, B69a, B69b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BS77]
[BS77]	(Browne+Savage, 1977)
Write:	<<[BS77] HHMM+DDdU>>
N:	2
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	Other QSO in Table 1 are PKS objects Paper III, see also Paper I: [BSB75] Paper II: [SBB76]
Ref:	=1977MNRAS.179p..65B
by	BROWNE I.W.A. , SAVAGE A.
	Mon. Not. R. Astron. Soc., 179, part no 16, 65-67 (1977)
	Redshift of southern quasars. III.
o	Table 1: <[BS77] 0149-474U>, <[BS77] 0154-512U>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BS85]
[BS85]	(Blair+Schild, 1985)
Write:	<<[BS85] N>> <<[BS85] A>>
N:	6+16
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Sources in CTB 80 field Format 'N' is for the closest X-ray position sources Map
Ref:	=1985ApL....24..189B
by	BLAIR W.P. , SCHILD R.E.
	Astrophys. Lett., 24, 189-195 (1985)
	Possible optical counterparts to the X-ray point source in the supernova remnant CTB 80.
o	Table 1: <[BS85] N> (Nos 1-3), <[BS85] A> (Nos A-P).
Ref:	=1998A&A...335..991O
by	O'SULLIVAN C. , SHEARER A., COLHOUN M., GOLDEN A., REDFERN M., BUTLER R., BESKIN G.M., NEIZVESTNY S.I., NEUSTROEV V.V., PLOKHOTNICHENKO V.L., DANKS A.
	Astron. Astrophys., 335, 991-994 (1998)
	A search for the optical counterpart of PSR B1951+32 in the supernova remnant CTB 80.
o	Table 3: <[BS85] N> (Nos 4-6) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BS88]
[BS88]	(Bothun+Schombert, 1988)
Write:	<<[BS88] ACO NNNN NN>>
N:	10+16+14
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Velocity of bound galaxies in ACO 2271, ACO 2589, ACO 2634.
in source:	ACO 2271
in source:	ACO 2589
in source:	ACO 2634
Ref:	=1988ApJ...335..617B
by	BOTHUN G.D. , SCHOMBERT J.M.
	Astrophys. J., 335, 617-628 (1988)
	Bound populations around cD galaxies.
o	Table 1: <[BS88] ACO 2271 NN> N=10 among (Nos 1-19). Table 2: <[BS88] ACO 2589 NN> N=16 among (Nos 1-40). Table 3: <[BS88] ACO 2634 NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BS94]
[BS94]	(Bohm+Solf, 1994)= (BS)
Write:	<<[BS94] A>>
N:	12
Object:	Component (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=12 emission components of T Tau
in source:	V* T Tau
Ref:	=1994ApJ...430..277B
by	BOHM K.-H. , SOLF J.
	Astrophys. J., 430, 277-290 (1994)
	A sub-arcsecond-scale spectroscopic study of the complex mass outflows in the vicinity of T Tauri.
o	<[BS94] A> (Nos A-F).
Ref:	=1999ApJ...523..709S
by	SOLF J. , BOHM K.-H.
	Astrophys. J., 523, 709-720 (1999)
	A deep long-slit spectroscopic study of the two bipolar outflows from the T Tauri binary system.
o	p.714: HH A and HH N = [RCL95] HH A and HH N.
o	Fig.2: <[BS94] A> (Nos G-L) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BS95]
[BS95]	(Bica+Schmitt, 1995)= (BS)
Write:	<<[BS95] NNN>>
N:	284
Object:	Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=247 objects, called 'BSNNN' by the authors, '[BS95] NNN' by SIMBAD. They are new Cl, Assoc, or Em. Neb. Updated in 2000AJ....119.1214B, Table 3. See also catalog in the SMC: BSDL.
in source:	Magellanic Clouds:SMC = SMC
in source:	Magellanic Clouds:Magellanic Bridge = Magellanic Bridge
Ref:	=1995ApJS..101...41B
by	BICA E.L.D. , SCHMITT H.R.
	Astrophys. J., Suppl. Ser., 101, 41-85 (1995)
	A revised and extended catalog of Magellanic system clusters, associations, and emission nebulae. I. Small Magellanic Cloud and Bridge.
o	Table 2: <[BS95] NNN> (Nos 1-247)
Ref:	=2000AJ....119.1214B
by	BICA E. , DUTRA C.M.
	Astron. J., 119, 1214-1224 (2000)
	Updating the census of star clusters in the Small Magellanic Cloud.
o	Table 3: <[BS95] NNN> (Nos 248-284) added.
=E=	Catalogue in electronic form as J/ApJS/101/41
=E=	Catalogue in electronic form as J/AJ/119/1214
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSA2001]
[BSA2001]	(Bechtold+Siemiginowska+Aldcroft+, 2001)
Write:	<<[BSA2001] QSO JHHMM+DDMM abs N.NNN>> <<[BSA2001] QSO JHHMM+DDMM abs N.NN>>
N:	5
Object:	DLA
Note:	Absorber systems in the line of sight of 3 QSOs. This reference is considered as a compilation.
Ref:	=2001ApJ...562..133B
by	BECHTOLD J. , SIEMIGINOWSKA A., ALDCROFT T.L., ELVIS M., DOBRZYCKI A.
	Astrophys. J., 562, 133-138 (2001)
	Chandra detection of X-ray absorption associated with a damped Lyα system.
o	Table 2, text: <[BSA2001] QSO J0057+1446 abs N.NNN> N=2, <[BSA2001] QSO J1130-1449 abs N.NNN> N=2, <[BSA2001] QSO J1333+1649 abs N.NN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSA2012]
[BSA2012]	(Burkert+Schartmann+Alig+, 2012)
Write:	<<[BSA2012] GN>>
N:	2
Object:	Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	VLT SINFONI observations of N=1 cloud discovered in Clenet et al. (2005A&A...439L...9C), and N=1 dense, dusty and ionized gas clump discovered in Gillessen et al. (2012Natur.481...51G).
in source:	NAME Galactic Center
Ref:	=2012ApJ...750...58B
by	BURKERT A. , SCHARTMANN M., ALIG C., GILLESSEN S., GENZEL R., FRITZ T.K., EISENHAUER F.
	Astrophys. J., 750, 58 (2012)
	Physics of the galactic center cloud G2, on its way toward the supermassive black hole.
o	Text: <[BSA2012] GN> (Nos G1-G2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSA2016]
[BSA2016]	(Bettinelli+Simioni+Aparicio+, 2016)
Write:	<<[BSA2016] lens>> <<[BSA2016] source>>
N:	1+1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	GTC OSIRIS spectroscopy of the lens and the source galaxies associated with the gravitational lens system IAC J010127.83-334319.6.
Ref:	=2016MNRAS.461L..67B
by	BETTINELLI M. , SIMIONI M., APARICIO A., HIDALGO S.L., CASSISI S., WALKER A.R., PIOTTO G., VALDES F.
	Mon. Not. R. Astron. Soc., 461L, 67-71 (2016)
	The Canarias Einstein ring: a newly discovered optical Einstein ring.
o	<IAC J010127.83-334319.6> N=1 = <NAME Canarias Einstein ring> N=1. <[BSA2016] lens> N=1. <[BSA2016] source> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BSAS
BSAS	(BATSE Spectral Analysis Software)= BATSE
Write:	<<BSAS YYMMDD SSSSSS>> <<BSAS YYMMDD_SSSSSS>> (not recognised by Simbad, but found in literature)
N:	16+30
Object:	(Gamma) (SIMBAD class: gammaBurst = Gamma-ray Burst)
Note:	Two first ref. with new Gamma Bursts, identified by the date, and time in seconds, format 'YYMMDD_SSSSSS'
Ref:	=1993ApJ...413..281B
by	BAND D. , MATTESON J., FORD L., SCHAEFER B., PALMER D., TEEGARDEN B., CLINE T., BRIGGS M., PACIESAS W., PENDLETON G., FISHMAN G., KOUVELIOTOU C., MEEGAN C., WILSON R., LESTRADE P.
	Astrophys. J., 413, 281-292 (1993)
	Batse observations of Gamma-ray burst spectra. I. Spectral diversity.
o	<BSAS YYMMDD_SSSSSS> N=16
Ref:	=1994ApJS...92..285S
by	SCHAEFER B.E. , TEEGARDEN B.J., FANTASIA S.F., PALMER D., CLINE T.L., MATTESON J.L., BAND D.L., FORD L.A., FISHMAN G.J., MEEGAN C.A., WILSON R.B., PACIESAS W.S., PENDLETON G.N., BRIGGS M.S., LESTRADE J.P.
	Astrophys. J., Suppl. Ser., 92, 285-310 (1994)
	BATSE spectroscopy catalog of bright γ-ray bursts.
o	<BSAS YYMMDD_SSSSS> N=30
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BSB2006]
[BSB2006]	(Beasley Srader+Brodie+, 2006)
Write:	<<[BSB2006] GCNN>>
N:	12
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	HST ACS archival data photometry and KECK LRIS spectroscopy of globular clusters in VCC 1087 galaxy.
in source:	VCC 1087
Ref:	=2006AJ....131..814B
by	BEASLEY M.A. , STRADER J., BRODIE J.P., CENARRO A.J., GEHA M.
	Astron. J., 131, 814-827 (2006)
	The globular cluster system of the Virgo dwarf elliptical galaxy VCC 1087.
o	Table 1: <[BSB2006] GCNN> N=12 among (Nos GC1 to GC26).
=E=	Catalogue in electronic form as J/AJ/131/814
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSB2007]
[BSB2007]	(Bower+Saul+Bloom+, 2007)
Write:	<<[BSB2007] JHHMMSS.ss+DDMMSS.ss>> <<[BSB2007] RT YYYYMMDD>>
N:	22+10
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA 5GHz and 8.4GHz multi-epoch observations. In format RT YYYYMMDD, RT stands for radiotransient.
Ref:	=2007ApJ...666..346B
by	BOWER G.C. , SAUL D., BLOOM J.S., BOLATTO A., FILIPPENKO A.V., FOLEY R.J., PERLEY D.
	Astrophys. J., 666, 346-360 (2007)
	Submillijansky transients in archival radio observations.
o	Tables 1, 2, 3: the transient sources are not in SIMBAD.
o	Tables 1-3: <[BSB2007] JHHMMSS.ss+DDMMSS.ss> N=12+8+2. Tables 2-3: <[BSB2007] RT YYYYMMDD> N=8+2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSB75]
[BSB75]	(Browne+Savage+Bolton, 1975)
Write:	<<[BSB75] HHMM+DDdW>>
N:	1
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	Others QSO in Table 1 are PKS objects Paper I, see also Paper II: [SBB76] Paper III: [BS77]
Ref:	=1975MNRAS.173p..87B
by	BROWNE I.W.A. , SAVAGE A., BOLTON J.G.
	Mon. Not. R. Astron. Soc., 173, part no 16, 87-91 (1975)
	Redshifts for southern quasars.
o	Table I: <[BSB75] 2320-035W>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BSC
BSC	(Bright * Catalog)
*****	Avoid the usage of BSC, prefer HR
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BSC2003]
[BSC2003]	(Barth+Sari+Cohen+, 2003)
Write:	<<[BSC2003] GRB 020813 abs N.NNN>>
N:	2
Object:	Absorber
Note:	LRIS spectropolarimetry at the Keck telescope of GRB 020813.
Ref:	=2003ApJ...584L..47B
by	BARTH A.J. , SARI R., COHEN M.H., GOODRICH R.W., PRICE P.A., FOX D.W., BLOOM J.S., SODERBERG A.M., KULKARNI S.R.
	Astrophys. J., 584, 47-51 (2003)
	Optical spectropolarimetry of the GRB 020813 afterglow.
o	<[BSC2003] GRB 020813 abs N.NNN> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSC2004]
[BSC2004]	(Borys+Scott+Chapman+, 2004)= (SMM)
Write:	<<[BSC2004] SMM JHHMMSS+DDMMSS>>
N:	39
Object:	(submm) (SIMBAD class: Galaxy)
Note:	Multiwavelength imaging of SCUBA submillitre sources. See also [BCH2002], [BCH2003].
in source:	NAME HDFN
Ref:	=2004MNRAS.355..485B
by	BORYS C. , SCOTT D., CHAPMAN S., HALPERN M., NANDRA K., POPE A.
	Mon. Not. R. Astron. Soc., 355, 485-503 (2004)
	The Hubble Deep Field North SCUBA Super-map - II. Multiwavelength properties.
o	Table 4: <[BSC2004] SMM JHHMMSS+DDMMSS> N=39.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSC2005]
[BSC2005]	(Bartkiewicz+Szymczak+Cohen+, 2005) (Not yet in Simbad)
Write:	<<[BSC2005] 1665 LHC A>> <<[BSC2005] 1665 RHC a>> <<[BSC2005] 1667 LHC A>> <<[BSC2005] 1667 RHC a>> <<[BSC2005] 1720 LHC A>> <<[BSC2005] 1720 RHC a>>
N:	50
Object:	OH Maser (SIMBAD class: Maser)
Note:	MERLIN polarization mapping of OH Masers at 1665, 1667 and 1720MHz toward the Cep A star-forming region.
in source:	NAME Cep A
Ref:	=2005MNRAS.361..623B
by	BARTKIEWICZ A. , SZYMCZAK M., COHEN R.J., RICHARDS A.M.S.
	Mon. Not. R. Astron. Soc., 361, 623-632 (2005)
	Magnetic field in Cepheus A as deduced from OH maser polarimetric observations.
o	Source 2300+638 = JVAS B2300+638.
o	Table 2: <[BSC2005] 1665 LHC A> (Nos A-Z), <[BSC2005] 1665 RHC a> (Nos a-p), <[BSC2005] 1667 LHC A> (Nos A-d), <[BSC2005] 1667 RHC a> (Nos a-b), <[BSC2005] 1720 LHC A> (No. A), <[BSC2005] 1720 RHC a> (No. a).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSC2007]
[BSC2007]	(Boris+Sodre+Cypriano+, 2007)= (QP)
Write:	<<[BSC2007] QP JHHMM+DDMM>>
N:	4
Object:	QSO Pair (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	Gemini GMOS spectroscopy of fields around 4 QSO pairs.
Ref:	=2007ApJ...666..747B
by	BORIS N.V. , SODRE L.Jr, CYPRIANO E.S., SANTOS W.A., MENDES DE OLIVEIRA C., WEST M.
	Astrophys. J., 666, 747-756 (2007)
	Searching high-redshift large-scale structures: photometry of four fields around quasar pairs at z ~ 1.
o	Table 2: <[BSC2007] QP JHHMM+DDMM> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSC2014]
[BSC2014]	(Beltran+Sanchez-Monge+Cesaroni+, 2014)
Write:	<<[BSC2014] A>>
N:	6
Object:	Core (SIMBAD class: denseCore = Dense Core)
Note:	ALMA 870µm continuum observations of N=6 cores toward the high-mass star-forming region G35.03+0.35.
in source:	GAL 035.03+00.35
Ref:	=2014A&A...571A..52B
by	BELTRAN M.T. , SANCHEZ-MONGE A., CESARONI R., KUMAR M.S.N., GALLI D., WALMSLEY C.M., ETOKA S., FURUYA R.S., MOSCADELLI L., STANKE T., VAN DER TAK F.F.S., VIG S., WANG K.-S., ZINNECKER H., ELIA D., SCHISANO E.
	Astron. Astrophys., 571A, 52-52 (2014)
	Filamentary structure and Keplerian rotation in the high-mass star-forming region G35.03+0.35 imaged with ALMA.
o	Table 3: <[BSC2014] A> (Nos A-F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSC2015]
[BSC2015]	(Berg+Skillman+Croxall+, 2015)
Write:	<<[BSC2015] NGC628+xxx.x+yyy.y>>
N:	64
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	LBT MODS observations of N=64 HI regions in NGC 628, as part of the CHemical Abundances Of Spirals (CHAOS) project. See also [CPB2015] for HII regions in NGC 5194, [CPB2016] for HII regions in NGC 5457, [BPS2020] for HII regions in NGC 3184, and [RSP2021] for HII regions in NGC 2403.
in source:	M 74 = NGC 628
Ref:	=2015ApJ...806...16B
by	BERG D.A. , SKILLMAN E.D., CROXALL K.V., POGGE R.W., MOUSTAKAS J., JOHNSON-GROH M.
	Astrophys. J., 806, 16 (2015)
	CHAOS I. Direct chemical abundances for H II regions in NGC 628.
o	Table 2: <[BSC2015] NGC628+xxx.x+yyy.y> N=64.
=E=	Catalogue in electronic form as <J/ApJ/806/16/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [BSC2017]
[BSC2017]	(Bennet+Sand+Crnojevic+, 2017)
Write:	<<[BSC2017] Dw NN>>
N:	38
Object:	LSB (SIMBAD class: LowSurfBrghtG = Low Surface Brightness Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Identification of N=38 low surface brightness dwarf candidates in the M101 group. Use of CFHTLS images.
in source:	M 101 = NGC 5457
Ref:	=2017ApJ...850..109B
by	BENNET P. , SAND D.J., CRNOJEVIC D., SPEKKENS K., ZARITSKY D., KARUNAKARAN A.
	Astrophys. J., 850, 109-109 (2017)
	Discovery of diffuse dwarf galaxy candidates around M101.
o	Table 1: <[BSC2017] Dw NN> (Nos 1-38).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSC84]
[BSC84]	(Bartel+Shapiro+Corey+, 1984)
Write:	<<[BSC84] 2021+614 A>>
N:	5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	N=5 components of Gopal 2021+614.
in source:	Gopal 2021+614
Ref:	=1984ApJ...279..116B
by	BARTEL N. , SHAPIRO I.I., COREY B.E., MARCAIDE J.M., ROGERS A.E.E., WHITNEY A.R., CAPPALLO R.J., KUHR H., GRAHAM D.A., BAATH L.B.
	Astrophys. J., 279, 116-121 (1984)
	The compact radio source 2021+614: simultaneous 2.3 and 8.3 GHz Mark III VLBI observations.
o	Table 1: <[BSC84] 2021+614 A> (Nos A-D).
Ref:	=2000A&A...360..887T
by	TSCHAGER W. , SCHILIZZI R.T., ROETTGERING H.J.A., SNELLEN I.A.G., MILEY G.K.
	Astron. Astrophys., 360, 887-895 (2000)
	The GHz-peaked spectrum radio galaxy 2021+614: detection of slow motion in a compact symmetric object.
o	p. 887 : Radio galaxy 1943+456 misprint for 1943+546 (CJ1 1943+546)
o	Fig.1: <[BSC84] 2021+614 A> (No. E) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSC90]
[BSC90]	(Barsony+Scoville+Schombert+, 1990)
Write:	<<[BSC90] Star A>> <<[BSC90] Cloudlet N>>
N:	2+5
Object:	* + Cloud (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Palomar 1.5m telescope optical photometry and OVRA 13CO(1-0) observations of the LkHA 101 environment. N=2 stars (A, B) and 5 molecular cloudlets.
Ref:	=1990ApJ...362..674B
by	BARSONY M. , SCOVILLE N.Z., SCHOMBERT J.M., CLAUSSEN M.J.
	Astrophys. J., 362, 674-690 (1990)
	The circumstellar environment of the emission-line star, LkHα 101.
o	Fig.1, Table 2: <[BSC90] Star A> (Nos A-B). Fig.15: <[BSC90] Cloudlet N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BSCC
BSCC	(Brorfelde Schmidt CCD Catalog)
Write:	<<BSCC NNNNNNNN>>
N:	13700000
Object:	* (SIMBAD class: Star)
Note:	CCD direct imaging observations 2000 - 2007; catalog of accurate positions (on ICRF) and V, R photometry, covering +49 to +90 deg Dec, about V=10 to 18 mag, observed with Brorfelde Schmidt Telescope (Denmark) in collaboration with Univ. of Copenhagen; new data, plan catalog release through CDS, paper in preparation for AJ. The authors prefer no space between the acronym and the 8 digit number, so the name would be exactly 12 characters long in all cases (with leading zeros, if any).
Auth.:	Norbert Zacharias U.S. Naval Observatory
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: BSCG
BSCG	(Bahcall+Soneira, Cluster of G)= (BAS) = (BS)
Write:	<<BSCG NNA>>
N:	19
Object:	Supercluster of G (SIMBAD class: SuperClG = Supercluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	also designated with the mean supercluster position 'HHMM+DDMM'
Ref:	=1984ApJ...277...27B
by	BAHCALL N.A. , SONEIRA R.M.
	Astrophys. J., 277, 27-37 (1984)
	A supercluster catalog.
o	Table 1: <BSCG NNA> (Nos 1-16, 12A-12C)
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: BSD
BSD	(Bergedorfer obs., Spektral Durchmusterung)= BSp = (Grn) = (SA)
Write:	<<BSD FFF-NNNN>>
N:	173599
Object:	Northern * (SIMBAD class: Star)
Note:	Lists for Northern Kapteyn selected areas, containing, for stars down to 13th photographic magnitude, the spectra from surveys with the Lippert astrograph of the Hamburg Observatory at Bergedorf, and the magnitudes from surveys of the Harvard College Observatory, determined by the Kapteyn Astronomical Laboratory of Groningen (Nos 001-0001 to 115-0619)
Ref:	=1935BSD...C01....0S
by	SCHWASSMANN A. , VAN RHIJN P.J.
	Hamburger Sternwarte Bergedorf, 1, 0-None (1935)
	Bergedorfer spektral-Durchmusterung der 115 Nordlichen Kapteynschen Eichfelder 1-19.
o	<BSD FF-NNNN>
Ref:	=1938BSD...C02....0S
by	SCHWASSMANN A. , VAN RHIJN P.J.
	Hamburger Sternwarte Bergedorf, 2, 0-None (1938)
	Bergedorfer Spektral-Durchmusterung der 115 Nordlichen Kapteynschen Eichfelder 20-43.
o	<BSD FF-NNNN>
Ref:	=1947BSD...C03....0S
by	SCHWASSMANN A. , VAN RHIJN P.J.
	Hamburger Sternwarte Bergedorf, 3, 0-None (1947)
	Bergedorfer Spektral-Durchmusterung der 115 Nordlichen Kapteyn Eichfelder 44-67.
o	<BSD FF-NNNN>
Ref:	=1951BSD...C04....0S
by	SCHWASSMANN A. , VAN RHIJN P.J.
	Hamburger Sternwarte Bergedorf, 4, 0-None (1951)
	Bergedorfer Spektral-Durchmusterung der 115 Nordlichen Kapteynschen Eichfelder 68-91.
o	<BSD FF-NNNN>
Ref:	=1953BSD...C05....0S
by	SCHWASSMANN A. , VAN RHIJN P.J.
	Hamburger Sternwarte Bergedorf, 5, 0-None (1953)
	Bergedorf Spektral-Durchmusterung der 115 Nordlichen Kapteynschen Eichfelder 92-115.
o	<BSD FFF-NNNN>
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BSD
BSD	(Bergedorfer obs., Spektral Durchmusterung)= (Pot) = PSD = SA
Write:	<<BSD FFF-NNNN>>
N:	66703
Object:	Southern * (SIMBAD class: Star)
Note:	Lists for Southern Kapteyn selected areas
Ref:	=1929POPot..27....1B
by	BECKER F.
	Publ. Astrophys. Obs. Potsdam, 27, 1-None (1929)
	Spektral-Durchmusterung der Kapteyn-Eichfelder des Sudhimmels. I. Pol und Zone -75°.
o	No. 66. Fields 200-206
o	<BSD FFF-NNNN> N=3639
Ref:	=1930POPot..27....1B
by	BECKER F.
	Publ. Astrophys. Obs. Potsdam, 27, 1-None (1930)
	Spektral-Durchmusterung der Kapteyn-Eichfelder des Sudhimmels. II. Zone -60°.
o	No. 89. Fields 188-189
o	<BSD FFF-NNNN> N=11753
Ref:	=1931POPot..27....1B
by	BECKER F.
	Publ. Astrophys. Obs. Potsdam, 27, 1-None (1931)
	Spektral-Durchmusterung der Kapteyn-Eichfelder des Sudhimmels. III. Zone -45°.
o	No. 90. Fields 164-187
o	<BSD FFF-NNNN> N=17730
Ref:	=1935POPot..28....1B
by	BRUCK H.
	Publ. Astrophys. Obs. Potsdam, 28, 1-None (1935)
	Spektral Durchmusterung der Kapteyn-Eichfelder des Sudhimmels. IV. Teil. Zone -30 Grad.
o	No. 91. Fields 140-163
o	<BSD FFF-NNNN> N=17045
Ref:	=1938POPot..28....1B
by	BECKER F.
	Publ. Astrophys. Obs. Potsdam, 28, 1-None (1938)
	Spektral-Durchmusterung der Kapteyn-Eichfelder des Sudhimmels. V. Zone -15°.
o	No. 92. Fields 115-139
o	<BSD FFF-NNNN> N=16536
Details on Acronym: [BSD2000]
[BSD2000]	(Bachev+Strigachev+Dimitrov, 2000) (Not yet in Simbad)
Write:	<<[BSD2000] Mkn NNN A>> <<[BSD2000] II Zw 1 A>> <<[BSD2000] Akn 120 A>>
N:	50
Object:	* (SIMBAD class: Star)
Note:	N=50 comparison stars in the field of 12 galaxies. Finding charts in Fig.2.
Ref:	=2000A&AS..147..175B
by	BACHEV R. , STRIGACHEV A., DIMITROV V.
	Astron. Astrophys., Suppl. Ser., 147, 175-180 (2000)
	VRI comparison stars for selected active galaxies.
o	Table 2: <[BSD2000] Mkn NNN A>, <[BSD2000] II Zw 1 A>, <[BSD2000] Akn 120 A>, N=50.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSD2005]
[BSD2005]	(Brodie+Strader+Denicolo+, 2005)= (Bro05)
Write:	<<[BSD2005] NN>>
N:	23
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Note:	Keck I LRIS spectroscopy of globular clusters in NGC 4365. See also [LBB2003] and [LBS2005].
in source:	NGC 4365
Ref:	=2005AJ....129.2643B
by	BRODIE J.P. , STRADER J., DENICOLO G., BEASLEY M.A., CENARRO A.J., LARSEN S.S., KUNTSCHNER H., FORBES D.A.
	Astron. J., 129, 2643-2653 (2005)
	Old globular clusters masquerading as young in NGC 4365?
o	Table 1: <[BSD2005] NN> (Nos 1-23).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSD2009]
[BSD2009]	(Brandl+Snijders+Den Brok+, 2009)
Write:	<<[BSD2009] PN>>
N:	6 (SIMBAD class: StarFormingReg = Star Forming Region)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRS observations of the Antennae galaxies.
in source:	NAME Antennae
Ref:	=2009ApJ...699.1982B
by	BRANDL B.R. , SNIJDERS L., DEN BROK M., WHELAN D.G., GROVES B., VAN DER WERF P., CHARMANDARIS V., SMITH J.D., ARMUS L., KENNICUTT R.C., HOUCK J.R.
	Astrophys. J., 699, 1982-2001 (2009)
	Spitzer-IRS study of the Antennae galaxies NGC 4038/39.
o	Table 2 : <[BSD2009] PN> (Nos P1-P6)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSD80]
[BSD80]	(Blair+St Clair Dinger+Dickinson, 1980)
Write:	<<[BSD80] HHMMSS.s+DDMMSS>> <<[BSD80] HHMMSS+DDMMSS>>
N:	6
Object:	H2O Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	Haystack observatory. New water masers detected in six sources.
in source:	SH 2-201
in source:	IRC +10374
in source:	SH 2-76 W
in source:	SH 2-76 E
in source:	SH 2-87
in source:	IRC +10523
Ref:	=1980AJ.....85..161B
by	BLAIR G.N. , ST CLAIR DINGER A., DICKINSON D.F.
	Astron. J., 85, 161-165 (1980)
	Interstellar and stellar water maser emission.
o	Table 1: <[BSD80] HHMMSS+DDMMSS> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSD96]
[BSD96]	(Blum+Sellgren+DePoy, 1996)
Write:	<<[BSD96] NNN>>
N:	214
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=214 stars in the Galactic Center
in source:	NAME Gal Center
Ref:	=1996ApJ...470..864B
by	BLUM R.D. , SELLGREN K., DEPOY D.L.
	Astrophys. J., 470, 864-881 (1996)
	JHKL photometry and the K-band luminosity function at the Galactic Center.
o	T.1, cross-id. col(2): GCIRS, MPE, OSU, Tam, NAME BSD WC9, NAME AF star, NAME AF NW, NAME AF NWB, F95 A, B, j From Figer Thesis, not in SIMBAD
o	Table 1: <[BSD96] NNN> (Nos 1-147), <GCIRS NNWA>, <GCIRS NNA> (Nos 2L, 6WB, 10EL, 12NB, 30B). <NAME AF NWB>. Table 1, col(2): <OSU CN> (Nos C1-C4), <OSU F1>, <OSU He1>
Ref:	=2003ApJ...597..323B
by	BLUM R.D. , RAMIREZ S.V., SELLGREN K., OLSEN K.
	Astrophys. J., 597, 323-346 (2003)
	Really cool stars and the star formation history at the Galactic Center.
o	F95 B from Foger Thesis not in Simbad
o	Table 2: <[BSD96] NNN> (Nos 148-214) added.
=E=	Catalogue in electronic form as J/ApJ/597/323
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSD98]
[BSD98]	(Bally+Sutherland+Devine+, 1998)= (HST)
Write:	<<[BSD98] NN>>
N:	43
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2, FOC and FOS observations of sources near tet01 Ori A, B, C
in source:	NAME Orion Nebula
Ref:	=1998AJ....116..293B
by	BALLY J. , SUTHERLAND R.S., DEVINE D., JOHNSTONE D.
	Astron. J., 116, 293-321 (1998)
	Externally illuminated young stellar environments in the Orion nebula: Hubble Space Telescope planetary camera and ultraviolet observations.
o	Table 3: <[BSD98] NN> (Nos 1-43).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BSDB
BSDB	(Binary Star DataBase) (Not yet in Simbad)
Write:	<<BSDB JHHMMSS.ss+DDMMSS.s:{s\|p\|c}NNNAAA{-}NNNAAA>>
N:	50000
Object:	Binary and multiple stars: components, pairs and systems
Note:	We present a new acronym, BSDB, developed for the Binary star database, and we would like to register it in the IAU Registry. We had to accept the challenge of construction of a satisfactory scheme in the course of development of the BDB, Binary star DataBase (http://bdb.inasan.ru, Malkov et al. 2013, Kaygorodov et al. 2012). BDB is constructed as a source combining comprehensive information on binary stars of all observational and evolutionary types. It provides the user with synthesis of data from a large variety of catalogues and databases of binaries of different types: visual, orbital, astrometric, interferometric, eclipsing, spectroscopic, X-ray, etc. The BDB contains all data from catalogues on more than 100,000 stellar systems of multiplicity 2 and more: positional, photometric, spectroscopic, orbital and astrophysical parameters are provided when available. Organization of the information is based on careful cross-identification of the objects.
Notes:	The major problem in constructing a database containing various types of data for binary and multiple stars is to establish proper links between objects and data originated from different sources. For the correct data-object connections in BDB, we introduce three categories of objects: System, Pair and Component. This approach is caused by the fact that each of these categories has its own set of observational data. Mass, radius, temperature, luminosity, etc. are Component characteristics (the same set of astrophysical parameters as a single star might have). A Pair consists of two gravitationally linked objects (any of them may also happen to be a pair). This category is characterized by another set of parameters: relative position of pair members at the celestial sphere (for visual binaries), orbital parameters like period and eccentricity (for orbital and spectroscopic binaries), combined magnitude (for photometrically unresolved binaries), etc. The observers of binaries usually deal with pairs, and consequently, catalogues of binaries consist of entries describing pairs. Finally, a System is characterized by general parameters such as age, metallicity, distance, kinematics, etc. Based on these categories of objects, we have developed and now use a new consistent scheme of designations of binary/multiple stars. The "BSDB" (Binary Star DataBase) abbreviation is used as the acronym (as we have checked with the Dictionary of Nomenclature of Celestial Objects, the "BDB" acronym is not available for registration). To form the designation, we take equatorial coordinates for the standard equinox of J2000.0 from the catalogues. Coordinates given in the catalogues are precise enough to specify them in the form of HHMMSS.ss+DDMMSS.s or HHMMSS.ss-DDMMSS.s. Then we add a specifier to distinguish systems, pairs, and components (s, p, and c, respectively). Finally, we indicate what component or pair is referred to using numerals and capital letters. It should be noted that the authors of WDS catalogue (Mason et al. 2001, http://ad.usno.navy.mil/wds/) include in the catalogue results of searches for substellar companions to nearby stars by high-contrast and high-angular-resolution imaging (e.g., Chauvin et al. 2010, 41 objects in the WDS 13447-6348 = TYC 9012-1005-1 system; Janson et al. 2011, 105 objects in the WDS 19062-0453 = lambda Aql system). At least some of the objects are background stars; however, they are also included in WDS and, consequently, in BDB. Another example of a high-multiplicity system in WDS is WDS 05387-6906 = 30 Dor = Tarantula Nebula. Digital speckle interferometry yields some 65 objects in this HII region in the LMC (Weigelt and Baier 1985). The usual capital-letter component designations (e.g., AB, AC, etc.) are insufficient to accommodate the very large number of companions in such systems, so upper/lower case combinations (A,Ca; A,Cb; etc.) were utilized in WDS. The lower-case letters here are not meant to indicate any sort of hierarchical structure within the system. Currently, 11 WDS systems have 30 or more components and, obviously, this number will increase. That is why we have decided to use numerals to identify components on the upper level of hierarchy. For other levels, we use capital letters A, B, etc. So, an example of the designation for some triple system would be as follows: J000144.48+590527.1:s J000144.48+590527.1:p1A-1B J000144.48+590527.1:c1A J000144.48+590527.1:c1B J000144.48+590527.1:p1-2 J000144.48+590527.1:c2 Note that there is no component "1" in the list. The cause is that "1" is not a star in this system but a pair of stars (1A-1B) and, respectively, it is described with parameters typical for a pair (say, orbital period) and not for a component. The coordinate part of a designation does not vary within the system (in spite of the fact that the components "1" and "2" can differ in coordinates). Indicating a component designation, we in general follow the WDS notation, but we substitute capital letters for digits (for the upper level of system hierarchy) and small letters and digits for capital letters (for other levels). Thus, we introduce BSDB J043306.62+240954.9:p1BA-1BB for the pair WDS 04331+2410 Ab1,2. The proposed system is extended to other types of binaries. Note that our principal source of photometric (eclipsing) binaries, GCVS Samus et al. 2013, http://www.sai.msu.ru/groups/cluster/gcvs/), has the same coordinate precision as WDS and CCDM (Dommanget and Nys 2002), and the principal catalogue of spectroscopic binaries, SB9, is even more precise (here coordinates should be truncated — not rounded — to form a designation). A newly discovered distant component will be designated by the next vacant digit. The solution of a component in two sub-components will lead to an appearance of two new designations for the subcomponents, with letters A and B in two subsequent positions (e.g., subcomponents 2A and 2B will appear when the component 2 is resolved). In the latter case, the resolved component designation (BSDB Jxxxxxx.xx+xxxxxx.x:c2) will be moved to the "outdated BSDB name" column, and a new designation for the pair (BSDB Jxxxxxx.xx+xxxxxx.x:p2A-2B) will be constructed. To provide BSDB numbers for all binary systems included in the BDB, we are working to appoint BSDB identifiers to binary and multiple stars of every observational type. For this purpose, we are compiling the general catalog of identifications of binaries, preliminarily named Identification List of Binaries, ILB. The ILB should include BSDB identifications for all binary systems included in the catalogs up to date, as well as leave such possibility open for the coming binary lists/catalogs/surveys. The most representative catalogues of binary systems (from wide to close pairs) are gradually connected to the ILB. If an object is encountered for the first time, a unique BSDB identifier is attributed to it. Objects that already exist in the previously investigated catalogues are appended to the corresponding ILB entries. New objects (pairs, components) included in stellar systems already existing in ILB lead to adjustments of the relevant sections of the catalog. ILB provides cross-identification with the following widely-used and/or binary identifiers: Name/Bayer/Flamsteed, HD, HIP, GCVS, DM (BD, CD, CPD), CCDM, WDS, ADS, IDS, SBC9, IGR, PSR. Cross-ID problems are solved at this stage, and to do it properly, all available information (positional, photometric and sometimes already contained in catalogues cross-identification) is taken into account. We believe that the principles underlaying BSDB identifier compilation do satisfy the "IAU Specifications concerning designations for astronomical radiation sources outside the solar system" (unlike, say, similarly coordinate-based WDS and CCDM names). Also, one can easily make sure that the problems typical for binary/multiple-star designation schemes are basically avoided by the BSDB. Kovaleva D., Malkov O., Kaygorodov P., Karchevskij A., Samus N. "BSDB: a new consistent designation scheme for identifying objects in binary and multiple stars" 2015, Baltic Astronomy, accepted Kovaleva D.A., Debray B., Kaygorodov P.V., Malkov O.Yu., Oblak E. "VO-accessible Binary star DataBase BDB" 2015, Astronomy and Computing, submitted
Ref:	=2012BaltA..21..309K
by	KAYGORODOV P. , DEBRAY B., KOLESNIKOV N., KOVALEVA D., MALKOV O.
	BaltA, 21, 309-318 (2012)
	The New Version of the Binary Star Database (bdb).
Ref:	=2014A&AT...28..235M Institute of Astronomy, Moscow
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: BSDL
BSDL	(Bica+Schmitt+Dutra+L. Oliveira)
Write:	<<BSDL NNNN>>
N:	3246
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Catalog of star clusters, associations and emission nebulae in the LMC See also catalog in the SMC: [BS95].
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1999AJ....117..238B
by	BICA E.L.D. , SCHMITT H.R., DUTRA C.M., OLIVEIRA H.L.
	Astron. J., 117, 238-246 (1999)
	A revised and extended catalog of Magellanic system clusters, associations, and emission nebulae. II. The Large Magellanic Cloud.
o	Table 2: <BSDL NNNN> (Nos 1-3246). Table 2: <[SL63] NNNA> (Nos 97A, 289A, 408A, 504A) added.
=E=	Catalogue in electronic form as J/AJ/117/238
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BSE2004]
[BSE2004]	(Bunker+Stanway+Ellis+, 2004)
Write:	<<[BSE2004] NNNNN>>
N:	57
Object:	G (SIMBAD class: Galaxy)
Note:	HST ACS observations of the HUDF. ID 'NNNNN' corresponds to authors catalogue ID, and 'STScI NNNNN' to the HUDF catalogue released by STScI, see UDF. Among the 57 objects, 54 are identified as galaxies.
in source:	NAME HUDF
Ref:	=2004MNRAS.355..374B
by	BUNKER A.J. , STANWAY E.R., ELLIS R.S., McMAHON R.G.
	Mon. Not. R. Astron. Soc., 355, 374-384 (2004)
	The star formation rate of the Universe at z~ 6 from the Hubble Ultra-Deep Field.
o	Table 1: <[BSE2004] NNNNN> N=53.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSE2008]
[BSE2008]	(Bradac+Schrabback+Erben+, 2008)
Write:	<<[BSE2008] A>> <<[BSE2008] AN>>
N:	9+25
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Stat:	is completely incorporated in Simbad
Note:	HST ACS and Chandra data of the field of the RX J1347.5-1145 cluster of galaxies.
Ref:	=2008ApJ...681..187B
by	BRADAC M. , SCHRABBACK T., ERBEN T., McCOURT M., MILLION E., MANTZ A., ALLEN S., BLANDFORD R., HALKOLA A., HILDEBRANDT H., LOMBARDI M., MARSHALL P., SCHNEIDER P., TREU T., KNEIB J.-P.
	Astrophys. J., 681, 187-196 (2008)
	Dark matter and baryons in the X-ray luminous merging galaxy cluster RX J1347.5-1145.
o	Table 1: each image in a system A is designated as AN in SIMBAD. Fig.6: Object z=4.08 = [CK2002] O47332-4511.
o	Table 1, Figs 1, 2: <[BSE2008] A> (Nos A-I), <[BSE2008] AN> N=25.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSE2009]
[BSE2009]	(Buchholz+Schoedel+Eckart+, 2009)
Write:	<<[BSE2009] NNNN>> <<[BSE2009] +xx.xx+yy.yy>>
N:	5914+35
Object:	* (SIMBAD class: Star)
Note:	ESO VLT NACO observations of the Galactic center star cluster.
Ref:	=2009A&A...499..483B
by	BUCHHOLZ R.M. , SCHOEDEL R., ECKART A.
	Astron. Astrophys., 499, 483-501 (2009)
	Composition of the Galactic center star cluster. Population analysis from adaptive optics narrow band spectral energy distributions.
o	typelist.dat: <[BSE2009] NNNN> (Nos 1-5914). Table 8: <[BSE2009] +xx.xx+yy.yy> N=35.
=E=	Catalogue in electronic form as J/A+A/499/483
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSE99]
[BSE99]	(Bezecourt+Soucail+Ellis+, 1999)
Write:	<<[BSE99] NN>>
N:	37
Object:	Arclet (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	N=37 arclets in ACO 370
in source:	ACO 370
Ref:	=1999A&A...351..433B
by	BEZECOURT J. , SOUCAIL G., ELLIS R.S., KNEIB J.-P.
	Astron. Astrophys., 351, 433-441 (1999)
	Lensed galaxies in Abell 370. II. The ultraviolet properties of arclets and the star formation rate at high redshift.
o	Offset positions, objects [BSE99] not in SIMBAD if no cross-id.
o	Table 1: <[BSE99] NN> (Nos 1-37).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSF2009]
[BSF2009]	(Brown+Smith+Ferguson+, 2009)
Write:	<<[BSF2009] JHHMMSS.ss+DDMMSS.ss>>
N:	460823
Object:	Unknown (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST ACS deep optical images in six fields of the Andromeda Galaxy.
in source:	M 31 = NGC 224
Ref:	=2009ApJS..184..152B
by	BROWN T.M. , SMITH E., FERGUSON H.C., GUHATHAKURTA P., KALIRAI J.S., KIMBLE R.A., RENZINI A., RICH R.M., SWEIGART A.V., VANDENBERG D.A.
	Astrophys. J., Suppl. Ser., 184, 152-157 (2009)
	Deep optical photometry of six fields in the Andromeda galaxy.
o	Table 2-7: <[BSF2009] JHHMMSS.ss+DDMMSS.ss> N=460823.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSF2012]
[BSF2012]	(Blom+Spitler+Forbes, 2012)
Write:	<<[BSF2012] ACS NN.NNNN>> <<[BSF2012] SCam NNNNN>>
N:	2255+5625
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	HST ACS and Subaru Suprime-Cam obervations of N=2255+5625 globular cluster candidates in NGC 4365.
in source:	NGC 4365
Ref:	=2012MNRAS.420...37B
by	BLOM C. , SPITLER L.R., FORBES D.A.
	Mon. Not. R. Astron. Soc., 420, 37-60 (2012)
	Wide-field imaging of NGC 4365's globular cluster system: the third subpopulation revisited.
o	catalog.dat: <[BSF2012] ACS NN.NNNN> N=2255, <[BSF2012] SCam NNNNN> N=5625.
=E=	Catalogue in electronic form as J/MNRAS/420/37
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSF97]
[BSF97]	(Brinkmann+Siebert+Feigelson+, 1997)
Write:	<<[BSF97] JHHMMSS.ss+DDMMSS.s>> <<[BSF97] JHHMMSS.s+DDMMSS>>
N:	1499
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT All-Sky Survey: Radio to X-ray properties of a large sample of mostly previously optically unidentified radio-loud X-ray sources
Ref:	=1997A&A...323..739B
by	BRINKMANN W. , SIEBERT J., FEIGELSON E.D., KOLLGAARD R.I., LAURENT-MUEHLEISEN S.A., REICH W., FUERST E., REICH P., VOGES W., TRUEMPER J., McMAHON R.
	Astron. Astrophys., 323, 739-748 (1997)
	Radio-loud AGN in the northern ROSAT All-Sky Survey. II. Multi-frequency properties of unidentified sources.
o	Objects in Table 4 are only RX in SIMBAD.
o	Tables 1-2: <[BSF97] JHHMMSS.ss+DDMMSS.s>, Tables 3-4: <[BSF97] JHHMMSS.s+DDMMSS> N=1499
=E=	Catalogue in electronic form as J/A+A/323/739
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSG2002]
[BSG2002]	(Beuther+Schilke+Gueth+, 2002)
Write:	<<[BSG2002] mmNa>>
N:	3+6
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	IRAM Plateau de Bure millimeter observations of IRAS 05358+3543.
in source:	IRAS 05358+3543
Ref:	=2002A&A...387..931B
by	BEUTHER H. , SCHILKE P., GUETH F., McCAUGHREAN M., ANDERSEN M., SRIDHARAN T.K., MENTEN K.M.
	Astron. Astrophys., 387, 931-943 (2002)
	IRAS 05358+3543: Multiple outflows at the earliest stages of massive star formation.
o	Fig.7, Table 3: <[BSG2002] mmN> (Nos mm1-mm3).
Ref:	=2007A&A...466.1065B
by	BEUTHER H. , LEURINI S., SCHILKE P., WYROWSKI F., MENTEN K.M., ZHANG Q.
	Astron. Astrophys., 466, 1065-1076 (2007)
	Interferometric multi-wavelength (sub)millimeter continuum study of the young high-mass protocluster IRAS 05358+3543.
o	Fig.2, Table 2: <[BSG2002] mmNa> (Nos mm1a, mm1b, mm2a to mm2d).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSG2004]
[BSG2004]	(Beuther+Schilke+Gueth, 2004)
Write:	<<[BSG2004] IRAS 20293+3952 mm N>> <<[BSG2004] IRAS 20293+3952 outflow A>>
N:	3+4
Object:	(mm) + Outflow (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	IRAM Plateau de Bure interferometer and 30m telescope observations of the region of IRAS 20293+3952.
in source:	IRAS 20293+3952
Ref:	=2004ApJ...608..330B
by	BEUTHER H. , SCHILKE P., GUETH F.
	Astrophys. J., 608, 330-340 (2004)
	Massive molecular outflows at high spatial resolution.
o	Fig.3, Table 3: <[BSG2004] IRAS 20293+3952 mm N> (Nos 1-3). Table 4: <[BSG2004] IRAS 20293+3952 outflow A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSG2005]
[BSG2005]	(Bresolin+Schaerer+Gonzalez Delgado+, 2005)
Write:	<<[BSG2005] NGC NNNN NN>>
N:	13+16+9+14+18
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	VLT FORS observations of HII regions in 5 galaxies.
in source:	NGC 1232
in source:	NGC 1365
in source:	NGC 2903
in source:	NGC 2997
in source:	NGC 5236
Ref:	=2005A&A...441..981B
by	BRESOLIN F. , SCHAERER D., GONZALEZ-DELGADO R.M., STASINSKA G.
	Astron. Astrophys., 441, 981-997 (2005)
	A VLT study of metal-rich extragalactic HII regions. I. Observations and empirical abundances.
o	Appendix A: the new QSO = EQ J033334.2-360523.8 in SIMBAD.
o	Table 3: <[BSG2005] NGC 1232 NN> N=13 among (Nos 2-15), <[BSG2005] NGC 1365 NN> N=16 among (Nos 3-17), <[BSG2005] NGC 2903 NN> N=9 among (Nos 2-14). Table 4: <[BSG2005] NGC 2997 NN> N=14 among (Nos 3-16), <[BSG2005] NGC 5236 NN> N=18 among (Nos 2-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSG2013]
[BSG2013]	(Bastian+Schweizer+Goudfrooij+, 2013)
Write:	<<[BSG2013] JHHMMSS.ss+DDMMSS.s>>
N:	12
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST WFC3 observations of N=12 young massive clusters in NGC 7252.
in source:	NGC 7252
Ref:	=2013MNRAS.431.1252B
by	BASTIAN N. , SCHWEIZER F., GOUDFROOIJ P., LARSEN S.S., KISSLER-PATIG M.
	Mon. Not. R. Astron. Soc., 431, 1252-1263 (2013)
	Luminosity profiles and sizes of massive star clusters in NGC 7252.
o	Table 2: <[BSG2013] JHHMSS.ss+DDMMSS.s> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSG2014]
[BSG2014]	(Bik+Stolte+Gennaro+, 2014)
Write:	<<[BSG2014] JHHMMSS.s+DDMMSS>>
N:	1033+1681+2220
Object:	(NIR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	LBT LUCI1 near-infrared observations of N=1033+1681+2220 sources in W3 Main.
in source:	W 3
Ref:	=2014A&A...561A..12B
by	BIK A. , STOLTE A., GENNARO M., BRANDNER W., GOULIERMIS D., HUSSMANN B., TOGNELLI E., ROCHAU B., HENNING T., ADAMO A., BEUTHER H., PASQUALI A., WANG Y.
	Astron. Astrophys., 561A, 12-12 (2014)
	Deep near-infrared imaging of W3 Main: constraints on stellar cluster formation.
o	jhk, hk, k: <[BSG2014] JHHMMSS.s+DDMMSS> N=1033+1681+2220.
=E=	Catalogue in electronic form as J/A+A/561/A12
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSG2015]
[BSG2015]	(Buddendiek+Schrabback+Greer+, 2015)
Write:	<<[BSG2015] ClG-JHHMMSS.s+DDMMSS>>
N:	44
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	WHT ACAM photometry and spectroscopy and LBT photometry of N=44 massive galaxy clusters with redshifts z>0.6. Use of ROSAT All Sky Survey data.
Ref:	=2015MNRAS.450.4248B
by	BUDDENDIEK A. , SCHRABBACK T., GREER C.H., HOEKSTRA H., SOMMER M., EIFLER T., ERBEN T., ERLER J., HICKS A.K., HIGH F.W., HILDEBRANDT H., MARRONE D.P., MORRIS R.G., MUZZIN A., REIPRICH T.H., SCHIRMER M., SCHNEIDER P., VON DER LINDEN A.
	Mon. Not. R. Astron. Soc., 450, 4248-4276 (2015)
	Optical and Sunyaev-Zel'dovich observations of a new sample of distant rich galaxy clusters in the ROSAT All Sky.
o	Table B1: <[BSG2015] ClG-JHHMMSS.s+DDMMSS> N=44.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSG89]
[BSG89]	(Braz+Scalise+Gregorio Hetem+, 1989)
Write:	<<[BSG89] LLL.ll+B.bb>>
N:	8
Object:	H2O Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	Table II: N=8 new H2O masers in the direction of IRAS sources.
Ref:	=1989A&AS...77..465B
by	BRAZ M.A. , SCALISE E., GREGORIO-HETEM J.C., MONTEIRO DO VALE J.L., GAYLARD M.
	Astron. Astrophys., Suppl. Ser., 77, 465-469 (1989)
	Search for water vapor masers in the direction of IRAS sources associated with HII regions and molecular clouds.
o	Table II: <[BSG89] LLL.ll+B.bb> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSH2000]
[BSH2000]	(Burkert+Stecklum+Henning+, 2000)
Write:	<<[BSH2000] NN>>
N:	32
Object:	(Near IR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Stat:	is completely incorporated in Simbad
Note:	Near infrared in Bran 192E nebula. Map in Fig.1a.
in source:	BRAN 192E
Ref:	=2000A&A...353..153B
by	BURKERT A. , STECKLUM B., HENNING T., FISCHER O.
	Astron. Astrophys., 353, 153-162 (2000)
	Multi-wavelength imaging of the peculiar Vela Molecular Ridge nebula BBW 192E.
o	p. 159 : IRAS 04302-2247 misprint for 04302+2247
o	Table 2: <[BSH2000] NN> (Nos 1-32).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSH2017]
[BSH2017]	(Bagley+Scarlata+Henry+, 2017)
Write:	<<[BSH2017] WISPNNNa>>
N:	7
Object:	LAE + G (SIMBAD class: Galaxy)
Note:	N=2 z∼6.5 LAEs and N=5 galaxies in the WISP survey.
Ref:	=2017ApJ...837...11B
by	BAGLEY M.B. , SCARLATA C., HENRY A., RAFELSKI M., MALKAN M., TEPLITZ H., DAI Y.S., BARONCHELLI I., COLBERT J., RUTKOWSKI M., MEHTA V., DRESSLER A., McCARTHY P., BUNKER A., ATEK H., GAREL T., MARTIN C.L., HATHI N., SIANA B.
	Astrophys. J., 837, 11-11 (2017)
	A high space density of luminous Lyman α emitters at z ~ 6.5.
o	Tables 2+4: <[BSH2017] WISPNNNa> N=2+5 among (Nos 302-379).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSI2001]
[BSI2001]	(Blanton+Sarazin+Irwin, 2001)
Write:	<<[BSI2001] NN>>
N:	49
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of NGC 1553.
in source:	NGC 1553
Ref:	=2001ApJ...552..106B
by	BLANTON E.L. , SARAZIN C.L., IRWIN J.A.
	Astrophys. J., 552, 106-119 (2001)
	Diffuse gas and low-mass X-ray binaries in the Chandra observation of the S0 galaxy NGC 1553.
o	Table 1: <[BSI2001] NN> (Nos 1-49).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSK2013]
[BSK2013]
Write:	<<[BSK2013] NN>>
N:	10
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=10 filamentary star forming regions. Use of SST GLIMPSE data.
Ref:	=2013MNRAS.435..663B
by	BHAVYA B. , SUBRAMANIAM A., KURIAKOSE V.C.
	Mon. Not. R. Astron. Soc., 435, 663-678 (2013)
	Study of young stellar objects and associated filamentary structures in the inner Galaxy.
o	Fig. 2, Table 1: <[BSK2013] NN> (Nos 1-10).
Details on Acronym: [BSL2001]
[BSL2001]	(Brown+Swigart+Lanz+, 2001)
Write:	<<[BSL2001] JHHMMSS.ssss+DDMMSS.sss>>
N:	295
Object:	* in Cl* (SIMBAD class: Star)
Note:	HST STIS observations.
in source:	NGC 2808
Ref:	=2001ApJ...562..368B
by	BROWN T.M. , SWEIGART A.V., LANZ T., LANDSMAN W.B., HUBENY I.
	Astrophys. J., 562, 368-393 (2001)
	Flash mixing on the white dwarf cooling curve: understanding hot horizontal branch anomalies in NGC 2808.
o	Table 2: <[BSL2001] JHHMMSS.ssss+DDMMSS.sss> N=295.
=E=	Catalogue in electronic form as J/ApJ/562/368
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSL2004]
[BSL2004]	(Barrientos+Schade+Lopez-Cruz+, 2004)
Write:	<<[BSL2004] JHHMMSS.s+DDMMSS.s>>
N:	8747
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Observations from the University of Warsaw 1.3m telescope at the Las Campanas observatory. Photometric observations of 8747 galaxies in the fields of 28 clusters with redshifts in the range 0.05<z<0.11
Ref:	=2004ApJS..153..397B
by	BARRIENTOS L.F. , SCHADE D., LOPEZ-CRUZ O., QUINTANA H.
	Astrophys. J., Suppl. Ser., 153, 397-409 (2004)
	Photometric and morphological properties of nearby cluster galaxies.
o	Table 2: <[BSL2004] JHHMMSS.s+DDMMSS.s> N = 8747.
=E=	Catalogue in electronic form as J/ApJS/153/397
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSL97]
[BSL97]	(Bade+Siebert+Lopez+, 1997)
Write:	<<[BSL97] RX J0911.4+0551 A>>
N:	3
Object:	QSO component (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	ROSAT All-Sky-Survey See also [BCL98]
in source:	RX J0911.0+0551
Ref:	=1997A&A...317L..13B
by	BADE N. , SIEBERT J., LOPEZ S., VOGES W., REIMERS D.
	Astron. Astrophys., 317, 13-None (1997)
	RX J0911.4+0551: A new multiple QSO selected from the ROSAT All-Sky Survey.
o	Table 1: <[BSL97] RX J0911.4+0551 A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSM2001]
[BSM2001]	(Bianchi+Scuderi+Massey+, 2001)= (CTIO) = (LB)
Write:	<<[BSM2001] CTIO-NNNN>> <<[BSM2001] LB-fN-NNN>>
N:	3232+765+260
Object:	* (SIMBAD class: Star)
Note:	HST WFPC2 observations of NGC 6822. Table 1: CTIO photometry. Table 3: WFPC2 photometry in 2 fields f1 and f2.
in source:	NGC 6822
Ref:	=2001AJ....121.2020B
by	BIANCHI L. , SCUDERI S., MASSEY P., ROMANIELLO M.
	Astron. J., 121, 2020-2031 (2001)
	The massive star content of NGC 6822: ground-based and Hubble space telescope photometry.
o	Table 1: <[BSM2001] CTIO-NNNN> (Nos 1-3232). Table 3: <[BSM2001] LB-f1-NNN> N=760, <[BSM2001] LB-f2-NNN> N=260.
=E=	Catalogue in electronic form as J/AJ/121/2020
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSM2002]
[BSM2002]	(Beuther+Schilke+Menten+, 2002)= (IRDC)
Write:	<<[BSM2002] HHMMm+DDMM N>>
N:	154+27
Object:	Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	Imaging of 1.2 mm dust continuum emission with the MAMBO bolometer array on IRAM 30m telescope, with follow-up CS and C34S observations with the 30m.
Ref:	=2002ApJ...566..945B
by	BEUTHER H. , SCHILKE P., MENTEN K.M., MOTTE F., SRIDHARAN T.K., WYROWSKI F.
	Astrophys. J., 566, 945-965 (2002)
	High-mass protostellar candidates. II. Density structure from dust continuum and CS emission.
o	(Erratum) erratum vol. 633, p.535 (2005)
o	Table 2: <[BSM2002] HHMMm+DDMM N> N=154.
Ref:	=2005ApJ...634L..57S
by	SRIDHARAN T.K. , BEUTHER H., SAITO M., WYROWSKI F., SCHILKE P.
	Astrophys. J., 634, 57-60 (2005)
	High-mass starless cores.
o	Table 1: <[BSM2002] HHMMm+DDMM NN> N=27 added.
=E=	Catalogue in electronic form as J/ApJ/566/945
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSM2007]
[BSM2007]	(Berger+Shin+Milchaey+, 2007)
Write:	<<[BSM2007] JHHMMSS.sss+DDMMSS.ss>>
N:	14
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Magellan-Clay 6.5m telescope Low Dispersion Survey Spectrograph observations of EDCC 493. This galaxy cluster is located within the error circle of GRB 050911.
in source:	EDCC 493
Ref:	=2007ApJ...660..496B
by	BERGER E. , SHIN M.-S., MULCHAEY J.S., JELTEMA T.E.
	Astrophys. J., 660, 496-503 (2007)
	Galaxy clusters associated with short GRBs. I. The fields of GRBs 050709, 050724, 050911, and 051221a.
o	Table 3: <[BSM2007] JHHMMSS.sss+DDMMSS.ss> N=14.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSM2010]
[BSM2010]	(Blundell+Schechter+Morgan+, 2010)
Write:	<<[BSM2010] J0816+5003 WN-W>> <<[BSM2010] J0816+5003 Lens>>
N:	4+1
Object:	Grav. lensed image + Grav. lens (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	MERLIN, MDM, WIYN, WHT, UKIRT and VLA observations of the northern lobe of the giant radio galaxy J0816+5003: two hot spots, each doubly lensed, and the lensing galaxy.
Ref:	=2010ApJ...723.1319B
by	BLUNDELL K.M. , SCHECHTER P.L., MORGAN N.D., JARVIS M.J., RAWLINGS S., TONRY J.L.
	Astrophys. J., 723, 1319-1324 (2010)
	A doubled double hot spot in J0816+5003 and the logarithmic slope of the lensing potential.
o	Table 1: <[BSM2010] J0816+5003 WN-W> (Nos N1-E, N1-W, N2-E, N2-W), <[BSM2010] J0816+5003 Lens> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSM2011]
[BSM2011]	(Barrado+Stelzer+Morales-Calderon)
Write:	<<[BSM2011] wNNN>> <<[BSM2011] wNNNw>> <<[BSM2011] wNNN{c\|z}>> <<[BSM2011] C69WI1-NNNNN>>
N:	164+205+10
Object:	(X) + (Opt) + (IR) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	XMM EPIC and OM, Calar Alto Omega2000, SST MIPS and IRAC observations. When there is ambuiguity in the optical or IR identification of an X-ray source, a letter is added at the end of the format wNNN to denote whether the optical or IR source is close to the center of the X-ray error box (c), or south (s), north (n), west (w), or east (e).
in source:	Cl Collinder 69
Ref:	=2011A&A...526A..21B
by	BARRADO D. , STELZER B., MORALES-CALDERON M., BAYO A., HUELAMO N., STAUFFER J.R., HODGKIN S., GALINDO F., VERDUGO E.
	Astron. Astrophys., 526A, 21-21 (2011)
	XMM-Newton investigations of the Lambda Orionis star-forming region (XILO). I. The young cluster Collinder 69.
o	Tables 3-6, 8-9: <[BSM2011] wNNNa> N=164+205 among (Nos e001-e112, w001-w052). Tables 11-12: <[BSM2011] C69WI1-NNNNN> N=8+2 among (Nos C69EI1-00790 to C69EI1-14609, C69WI1-09288, C69WI1-14892).
=E=	Catalogue in electronic form as J/A+A/526/A21
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSM2016]
[BSM2016]	(Baran+Smolcic+Milakovic+, 2016)
Write:	<<[BSM2016] VTANN>>
N:	10
Object:	Galaxy overdense structure (SIMBAD class: ClG_Candidate = Cluster of Galaxies Candidate)
Note:	N=10 galaxy overdense structures found when applying Voronoi tessellation analysis (VTA) in the field of the first supercluster discovered in the XXL project.
Ref:	=2016A&A...592A...8B
by	BARAN N. , SMOLCIC V., MILAKOVIC D., NOVAK M., DELHAIZE J., GASTALDELLO F., RAMOS-CEJA M.E., PACAUD F., BOURKE S., CARILLI C.L., ETTORI S., HALLINAN G., HORELLOU C., KOULOURIDIS E., CHIAPPETTI L., MIETTINEN O., MELNYK O., MOOLEY K., PIERRE M., POMPEI E., SCHINNERER E.
	Astron. Astrophys., 592A, 8-8 (2016)
	The XXL Survey. IX. Optical overdensity and radio continuum analysis of a supercluster at z = 0.43.
o	Table 2: <VLA-XXL NNN> (Nos 1-155). Fig. 7, Table 3: <[BSM2016] VTANN> (Nos VTA01-VTA10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSM2020]
[BSM2020]	(Bodensteiner+Sana+Mahy+, 2020)= ([BSM2020a])
Write:	<<[BSM2020] NNN>>
N:	278+97
Object:	* (SIMBAD class: Star)
Note:	VLT MUSE observations of N=278+340 stars in the core of NGC 330.
in source:	Magellanic Clouds:SMC:NGC 330 = NGC 330
Ref:	=2020A&A...634A..51B
by	BODENSTEINER J. , SANA H., MAHY L., PATRICK L.R., DE KOTER A., DE MINK S.E., EVANS C.J., GOTBERG Y., LANGER N., LENNON D.J., SCHNEIDER F.R.N., TRAMPER F.
	Astron. Astrophys., 634A, 51-51 (2020)
	The young massive SMC cluster NGC 330 seen by MUSE. I. Observations and stellar content.
o	Table D.1: <[BSM2020] NNN> N=278 among (Nos 20-739).
Ref:	=2021A&A...652A..70B
by	BODENSTEINER J. , SANA H., WANG C., LANGER N., MAHY L., BANYARD G., DE KOTER A., DE MINK S.E., EVANS C.J., GOTBERG Y., PATRICK L.R., SCHNEIDER F.R.N., TRAMPER F.
	Astron. Astrophys., 652A, 70-70 (2021)
	The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population.
o	Table C.1: <[BSM2020] NNN> N=97 among (Nos 10-732) added.
=E=	Catalogue in electronic form as <J/A+A/634/A51/>
=E=	Catalogue in electronic form as <J/A+A/652/A70/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSM2020a]
[BSM2020a]	(Bodensteiner+Sana+Mahy+, 2020) (Not yet in Simbad)
*****	Avoid the usage of [BSM2020a], prefer [BSM2020]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSM2020b]
[BSM2020b]	(Bahramian+Strader+Miller-Jones+, 2020)
Write:	<<[BSM2020b] CXOU JHHMMSS.ss+DDMMSS.s>>
N:	1667
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS observations of N=1667 X-ray sources in 38 Galactic globular clusters.
Ref:	=2020ApJ...901...57B
by	BAHRAMIAN A. , STRADER J., MILLER-JONES J.C.A., CHOMIUK L., HEINKE C.O., MACCARONE T.J., POOLEY D., SHISHKOVSKY L., TUDOR V., ZHAO Y., LI K.L., SIVAKOFF G.R., TREMOU E., BUCHNER J.
	Astrophys. J., 901, 57-57 (2020)
	The MAVERIC survey: Chandra/ACIS catalog of faint X-ray sources in 38 Galactic globular clusters.
o	Table A1: <[BSM2020b] CXOU JHHMMSS.ss+DDMMSS.s> N=1667.
=E=	Catalogue in electronic form as <J/ApJ/901/57/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSM99]
[BSM99]	(Brosch+Shara+MacKenty+, 1999)
Write:	<<[BSM99] NNNa>>
N:	275
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 UV observations in the LMC. See also [PHC98]
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1999AJ....117..206B
by	BROSCH N. , SHARA M., MacKENTY J., ZUREK D., McLEAN B.
	Astron. J., 117, 206-224 (1999)
	Far-ultraviolet imaging of the field star population in the Large Magellanic Cloud with the Hubble space telescope.
o	Tables 2, 3: <[BSM99] NNNa> N=275 among (Nos 1-377).
=E=	Catalogue in electronic form as J/AJ/117/206
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSN2006]
[BSN2006]	(Baba+Sato+Nagashima+, 2006)
Write:	<<[BSN2006] NN>> <<[BSN2006] R>>
N:	31+5
Object:	Protostar + Cluster of * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	NIR survey of the Vela C Cloud at the IRSF 1.4m telescope at the South African Astronomical Observatory in Sutherland. Protostar candidates are selected on the base of positional coincidences with MSX5C and IRAS sources. 5 stellar clusters are also found.
in source:	VMR C
Ref:	=2006AJ....132.1692B
by	BABA D. , SATO S., NAGASHIMA C., NISHIYAMA S., KATO D., HABA Y., NAGATA T., NAGAYAMA T., TAMURA M., SUGITANI K.
	Astron. J., 132, 1692-1706 (2006)
	Deep near-infrared imaging toward the Vela molecular ridge C. II. New protostars and embedded clusters in Vela C.
o	Table 1: <[BSN2006] NN> (Nos 1-31). Table 3: <[BSN2006] R> (Nos I-V).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSN97]
[BSN97]	(Beekman+Shahbaz+Naylor+, 1997)
Write:	<<[BSN97] Comparison star>> <<[BSN97] Standard N>>
N:	1+2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	UKIRT observations. Comparison and standard stars in the field of GRO J0422+32. See also [CI95].
Ref:	=1997MNRAS.290..303B
by	BEEKMAN G. , SHAHBAZ T., NAYLOR T., CHARLES P.A., WAGNER R.M., MARTINI P.
	Mon. Not. R. Astron. Soc., 290, 303-312 (1997)
	The mass of the black hole in the low-inclination LMXB transient system GRO J0422 + 32 (=Nova Persei 1992).
o	[BSN97] Standard 2 is not the same star as [CI95] 2.
o	Table 2: <[BSN97] Comparison star> N=1, <[BSN97] Standard N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BSNS
BSNS	(Boyle+Smriglio+Nandy+Straizys)
Write:	<<BSNS NNN>>
N:	193
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1990A&AS...86..395B
by	BOYLE R.P. , SMRIGLIO F., NANDY K., STRAIZYS V.
	Astron. Astrophys., Suppl. Ser., 86, 395-401 (1990)
	CCD photometry in the Vilnius photometric system. II. Region in Sagitta.
o	<BSNS NNN> N=193
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BSNSN
BSNSN	(Boyle+Smriglio+Nandy+Straizys, North)
Write:	<<BSNSN NNN>>
N:	122
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table IV: Lyra North *
in source:	NAME Lyra
Ref:	=1990A&AS...84....1B
by	BOYLE R.P. , SMRIGLIO F., NANDY K., STRAIZYS V.
	Astron. Astrophys., Suppl. Ser., 84, 1-10 (1990)
	CCD photometry in the Vilnius photometric system. I. Region in Lyra.
o	Table III: <BSNSN NNN> (Nos 1-122). Table IV: <BSNSS NNN> (Nos 1-109).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BSNSS
BSNSS	(Boyle+Smriglio+Nandy+Straizys, South)
Write:	<<BSNSS NNN>>
N:	109
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table IV: Lyra South *
in source:	NAME Lyra
Ref:	=1990A&AS...84....1B
by	BOYLE R.P. , SMRIGLIO F., NANDY K., STRAIZYS V.
	Astron. Astrophys., Suppl. Ser., 84, 1-10 (1990)
	CCD photometry in the Vilnius photometric system. I. Region in Lyra.
o	Table III: <BSNSN NNN> (Nos 1-122). Table IV: <BSNSS NNN> (Nos 1-109).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BSO
BSO	(Blue Stellar Obj.)
*****	Avoid the usage of BSO, prefer [A76]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BSO
BSO	(Blue Stellar Obj.)
*****	Avoid the usage of BSO, prefer [A77]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BSO
BSO	(Blue Stellar Obj.)
*****	Avoid the usage of BSO, prefer [A81b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BSO
BSO	(Blue Stellar Obj.)
*****	Avoid the usage of BSO, prefer [AS79]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BSO
BSO	(Blue Stellar Obj.)
Write:	<<BSO NN>>
N:	31
Object:	BSO (SIMBAD class: blue = Blue Object)
Stat:	is completely incorporated in Simbad
Ref:	=1965ApJ...142..412S
by	SANDAGE A. , VERON P.
	Astrophys. J., 142, 412-414 (1965)
	Photometric results of a special survey for interlopers.
o	Table 1: <BSO NN> (Nos 1-31)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BSp
BSp	(Bergedorfer obs., Spektral)
*****	Avoid the usage of BSp, prefer BSD
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BSP2001]
[BSP2001]	(Blum+Schaerer+Pasquali+, 2001)
Write:	<<[BSP2001] NN>>
N:	34
Object:	* in Cl* (SIMBAD class: EmLine* = Emission-line Star)
in source:	NAME Arches Cluster
Ref:	=2001AJ....122.1875B
by	BLUM R.D. , SCHAERER D., PASQUALI A., HEYDARI-MALAYERI M., CONTI P.S., SCHMUTZ W.
	Astron. J., 122, 1875-1887 (2001)
	2 micron narrowband adaptive optics imaging in the Arches cluster.
o	Table 2: <[BSP2001] NN> (Nos 1-34).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSP2003]
[BSP2003]	(Becker+Swartz+Pavlov+, 2003)
Write:	<<[BSP2003] NN>>
N:	46
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of the globular cluster M28.
in source:	M 28 = NGC 6626
Ref:	=2003ApJ...594..798B
by	BECKER W. , SWARTZ D.A., PAVLOV G.G., ELSNER R.F., GRINDLAY J., MIGNANI R., TENNANT A.F., BACKER D., PULONE L., TESTA V., WEISSKOPF M.C.
	Astrophys. J., 594, 798-811 (2003)
	Chandra X-ray Observatory observations of the globular cluster M 28 and its millisecond pulsar PSR B1821-24.
o	Table 3: <[BSP2003] NN> (Nos 1-46).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSP2005]
[BSP2005]	(Belsole+Sauvageot+Pratt+, 2005)
Write:	<<[BSP2005] BGN>>
N:	3
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	MPG-ESO 2.2m telescope optical map and X-ray properties from XMM-Newton observations. N=3 Brightest Galaxies (BG in the format) in the cluster.
in source:	ACO 3921
Ref:	=2005A&A...430..385B
by	BELSOLE E. , SAUVAGEOT J.-L., PRATT G.W., BOURDIN H.
	Astron. Astrophys., 430, 385-397 (2005)
	An XMM-Newton observation of A3921: An off-axis merger.
o	Fig.1: <[BSP2005] BGN> (Nos BG1, BG2, BG3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSP2010]
[BSP2010]	(Begum+Stanimirovic+Peek+, 2010)
Write:	<<[BSP2010] NN>>
N:	96
Object:	HI Cloud (SIMBAD class: Cloud)
Note:	N=96 compact HI clouds found in the Galactic Arecibo L-band Feed Array HI (GALFA-HI) survey.
Ref:	=2010ApJ...722..395B
by	BEGUM A. , STANIMIROVIC S.Z., PEEK J.E., BALLERING N.P., HEILES C., DOUGLAS K.A., PUTMAN M., GIBSON S.J., GRCEVICH J., KORPELA E.J., LEE M.-Y., SAUL D., GALLAGHER III J.S.
	Astrophys. J., 722, 395-411 (2010)
	Compact H I clouds from the GALFA-H I survey.
o	Table 1: <[BSP2010] NN> (Nos 1-96).
=E=	Catalogue in electronic form as <J/ApJ/722/395/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSP2011]
[BSP2011]	(Billot+Schisano+Pestalozzi+, 2011)
Write:	<<[BSP2011] NN>>
N:	21
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	Herschel SDP observations of two target fields from the Hi-GAL survey. Search for clusters of YSO.
Ref:	=2011ApJ...735...28B
by	BILLOT N. , SCHISANO E., PESTALOZZI M., MOLINARI S., NORIEGA-CRESPO A., MOTTRAM J.C., ANDERSON L.D., ELIA D., STRINGFELLOW G., THOMPSON M.A., POLYCHRONI D., TESTI L.
	Astrophys. J., 735, 28 (2011)
	Clustering properties of far-infrared sources in Hi-GAL science demonstration phase fields.
o	Table 2: <[BSP2011] NN> (Nos 1-21).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSP2011b]
[BSP2011b]	(Belloche+Schuller+Parise+, 2011)
Write:	<<[BSP2011b] Ngcl NNN>> <<[BSP2011b] Nadd N>> <<[BSP2011b] Cha1-CNN>> <<[BSP2011b] Cha1-SNN>>
N:	204 (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	APEX LABOCA 870µm observations of Chamaeleon I.
in source:	NAME Cha I
Ref:	=2011A&A...527A.145B
by	BELLOCHE A. , SCHULLER F., PARISE B., ANDRE P., HATCHELL J., JORGENSEN J.K., BONTEMPS S., WEISS A., MENTEN K.M., MUDERS D.
	Astron. Astrophys., 527A, 145-145 (2011)
	The end of star formation in Chamaeleon I? A LABOCA census of starless and protostellar cores.
o	Paragraph 2.1 IRAS 13134-6264 is a misprint for IRAS 13134-6242.
o	<[BSP2011b] Ngcl NNN>, <[BSP2011b] Nadd N>, <[BSP2011b] Cha1-CNN>, <[BSP2011b] Cha1-SNN> N=204.
=E=	Catalogue in electronic form as <J/A+A/527/A145/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSP2012]
[BSP2012]	(Bhatt+Sagar+Pandey, 2012)
Write:	<<[BSP2012] NNNN>>
N:	2261
Object:	* (SIMBAD class: Star)
Note:	UBVRI photometric observations of Cl Stock 18 with the 104-cm Sampurnanand telescope (Nainital). Use of archival 2MASS, IRAS, MSX, AKARI data.
in source:	Cl Stock 18
Ref:	=2012NewA...17..160B
by	BHATT H. , SAGAR R., PANDEY J.-C.
	NewA, 17, 160-166 (2012)
	Stellar contents and star formation in the young cluster Stock 18.
o	Paragraph 2.1: BD+63 2092p is a misprint for BD+63 2093p.
o	Table 2: <[BSP2012] NNNN> (Nos 1-2261).
=E=	Catalogue in electronic form as J/other/NewA/17.160
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSP2020]
[BSP2020]	(Byun+Sheen+Park+, 2020)
Write:	<<[BSP2020] N1291-DWNN>>
N:	15
Object:	Poss. Dwarf G (SIMBAD class: Galaxy_Candidate = Galaxy Candidate)
Stat:	is completely incorporated in Simbad
Note:	KMTNet 1.6 m telescopes observations of N=15 dwarf galaxy candidates in the field of the NGC 1291 system.
Ref:	=2020ApJ...891...18B
by	BYUN W. , SHEEN Y.-K., PARK H.S., HO L.C., LEE J.H., KIM S.C., JEONG H., PARK B.-G., SEON K.-I., LEE Y., LEE Y., CHA S.-M., KO J., KIM M.
	Astrophys. J., 891, 18-18 (2020)
	KMTNet nearby galaxy survey II. Searching for dwarf galaxies in deep and wide-field images of the NGC 1291 system.
o	Fig. 1, Table 2: <[BSP2020] N1291-DWNN> (Nos DW1-DW15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSP2022]
[BSP2022]	(Bell+Smercina+Price+, 2022)
Write:	<<[BSP2022] M81-dw JHHMM+DDMM>>
N:	8
Object:	Poss. Dwarf G (SIMBAD class: Galaxy_Candidate = Galaxy Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=8 dwarf galaxy candidates in the field of M81. Use of Subaru Hyper SuprimeCam data.
in source:	NGC 3031 = M 81
Ref:	=2022ApJ...937L...3B
by	BELL E.F. , SMERCINA A., PRICE P.A., D'SOUZA R., BAILIN J., DE JONG R.S., GOZMAN K., JANG I.S., MONACHESI A., GNEDIN O.Y., SLATER C.T.
	Astrophys. J., 937L, 3 (2022)
	Ultrafaint Dwarf Galaxy Candidates in the M81 Group: Signatures of Group Accretion.
o	Fig. 3, Table 1: <[BSP2022] M81-dw JHHMM+DDMM> N=8.
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [BSR2006]
[BSR2006]	(Becker+Sargent+Rauch+, 2006)
Write:	<<[BSR2006] QSO JHHMM+DDMM abs N.NNNN>>
N:	6
Object:	Absorber
Note:	O(I) systems of absorption in the spectra of 3 SDSS QSOs taken with Keck HIRES.
Ref:	=2006ApJ...640...69B
by	BECKER G.D. , SARGENT W.L.W., RAUCH M., SIMCOE R.A.
	Astrophys. J., 640, 69-80 (2006)
	Discovery of excess O I absorption toward the z=6.42 QSO SDSS J1148+5251.
o	Table 2: Only z(sys) are in SIMBAD, not z of components of each system.
o	Table 2: <[BSR2006] QSO JHHMM+DDMM abs N.NNNN> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSR2016]
[BSR2016]	(Baronchelli+Scarlata+Rodighiero+, 2016)= ([BSR2016a]) (Not yet in Simbad)
Write:	<<[BSR2016] NNNNNN>>
N:	341066
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Multiwavelength IRAC-based catalog of N=341066 sources, as part of the Spitzer-IRAC/MIPS Extragalactic survey (SIMES) in the South Ecliptic Pole (SEP) field.
in source:	NAME SEP
Ref:	=2016ApJS..223....1B
by	BARONCHELLI I. , SCARLATA C., RODIGHIERO G., FRANCESCHINI A., CAPAK P.L., MEI S., VACCARI M., MARCHETTI L., HIBON P., SEDGWICK C., PEARSON C., SERJEANT S., MENENDEZ-DELMESTRE K., SALVATO M., MALKAN M., TEPLITZ H.I., HAYES M., COLBERT J., PAPOVICH C., DEVLIN M., KOVACS A., SCOTT K.S., SURACE J., KIRKPATRICK J.D., ATEK H., URRUTIA T., SCOVILLE N.Z., TAKEUCHI T.T.
	Astrophys. J., Suppl. Ser., 223, 1-1 (2016)
	The Spitzer-IRAC/MIPS extragalactic survey (SIMES) in the South Ecliptic Pole field.
o	catalog.dat: <[BSR2016] NNNNNN> (Nos 1-341066).
=E=	Catalogue in electronic form as <J/ApJS/223/1/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSR2016a]
[BSR2016a]	(Baronchelli+Scarlata+Rodighiero+, 2016) (Not yet in Simbad)
*****	Avoid the usage of [BSR2016a], prefer [BSR2016]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSR2016b]
[BSR2016b]	(Balog+Siegler+Rieke+, 2016)
Write:	<<[BSR2016b] NNN>>
N:	295
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	CTIO 1.5m telescope, AAT AAOmega, and Spitzer IRAC and MIPS observations of N=295 stars in the open stellar cluster IC 2395.
in source:	IC 2395
Ref:	=2016ApJ...832...87B
by	BALOG Z. , SIEGLER N., RIEKE G.H., KISS L.L., MUZEROLLE J., GUTERMUTH R.A., BELL C.P.M., VINKO J., SU K.Y.L., YOUNG E.T., GASPAR A.
	Astrophys. J., 832, 87-87 (2016)
	Protoplanetary and transitional disks in the open stellar cluster IC 2395.
o	Tables 3-4: <[BSR2016b] NNN> (Nos 1-295).
=E=	Catalogue in electronic form as <J/ApJ/832/87/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSR99]
[BSR99]	(Bonfanti+Simien+Rampazzo+, 1999)
Write:	<<[BSR99] HCG NNa nN>>
N:	2+2
Object:	Nucleus (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	The galaxies HCG 67a and HCG 74a have 2 nucleus n1 and n2.
in source:	HCG 67a
in source:	HCG 74a
Ref:	=1999A&AS..139..483B
by	BONFANTI P. , SIMIEN F., RAMPAZZO R., PRUGNIEL P.
	Astron. Astrophys., Suppl. Ser., 139, 483-490 (1999)
	Kinematics of early-type galaxies in compact groups. HCG 67, HCG 74, and HCG 79.
o	Text: <[BSR99] HCG 67a aN> (Nos n1-n2), <[BSR99] HCG 74a aN> (Nos n1-n2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BSS
BSS	(Bolton+Stanley+Slee)= (B2)
Write:	<<BSS NNN>>
N:	104
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1954AuJPh...7..110B
by	BOLTON J.G. , STANLEY G.J., SLEE O.B.
	Australian J. Phys., 7, 110-129 (1954)
	Galactic radiation at radio frequencies. VIII. Discrete sources at 1OO Mc/s between declinations +50° and -50°.
o	<BSS NNN> N=104 among 123
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BSS
BSS	(Biurakan obs., Second Survey)
**	catalog: use SBSG
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BSS
BSS	(Biurakan obs., Second Survey)
**	catalog: use SBSS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BSS2003]
[BSS2003]	(Beuther+Schilke+Stanke, 2003)
Write:	<<[BSS2003] mmN>> <<[BSS2003] Outflow A>> <<[BSS2003] H2 NN>>
N:	6+7+12
Object:	(mm) + Part of Cloud (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	IRAM interferometer and Calar Alto observations of the star-forming region IRAS 19410+2336. N=6 mm sub-sources. See also [BSW2004].
in source:	IRAS 19410+2336
Ref:	=2003A&A...408..601B
by	BEUTHER H. , SCHILKE P., STANKE T.
	Astron. Astrophys., 408, 601-610 (2003)
	Multiple outflows in IRAS 19410+2336.
o	IRAS 20126+2104 is a misprint for 20126+4104.
o	Table 1: <[BSS2003] mmN> (Nos mm1 to mm6). Figs: <[BSS2003] Outflow A> (Nos A-G). Fig.3: <[BSS2003] H2 NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSS2004]
[BSS2004]	(Bonanos+Stanek+Szentgyorgyi+, 2004)
Write:	<<[BSS2004] Draco JHHMMSS.s+DDMMSS.s>>
N:	146+17
Object:	RR Lyr + V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	Fred Lawrence Whipple Observatory 1.2m telescope observations of the Draco dwarf galaxy. N=146 RR Lyrae stars (Table 1) and 17 other V* (Table 2).
in source:	NAME Draco Dwarf Galaxy
Ref:	=2004AJ....127..861B
by	BONANOS A.Z. , STANEK K.Z., SZENTGYORGYI A.H., SASSELOV D.D., BAKOS G.A.
	Astron. J., 127, 861-867 (2004)
	The RR Lyrae distance to the Draco dwarf spheroidal galaxy.
o	(Erratum) errata vol. 133, p. 756 (2007), vol. 136, p. 896 (2008)
o	Tables 1, 2: cross-id BS = [BS61] NNN in SIMBAD.
o	Tables 1, 2: <[BSS2004] Draco JHHMMSS.s+DDMMSS.s> N=146+17.
=E=	Catalogue in electronic form as J/AJ/127/861
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSS2005]
[BSS2005]	(Butler+Sakamoto+Suzuki+, 2005)
Write:	<<[BSS2005] N>>
Object:	(X) + * (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra sources in the error box of GRB 030723: Source 2 is a background USNO star.
Ref:	=2005ApJ...621..884B
by	BUTLER N.R. , SAKAMOTO T., SUZUKI M., KAWAI N., LAMB D.Q., GRAZIANI C., DONAGHY T.Q., DULLIGHAN A., VANDERSPEK R., CREW G.B., FORD P., RICKER G., ATTEIA J.-L., YOSHIDA A., SHIRASAKI Y., TAMAGAWA T., TORII K., MATSUOKA M., FENIMORE E.E., GALASSI M., DOTY J., VILLASENOR J., PRIGOZHIN G., JERNIGAN J.G., BARRAUD C., BOER M., DEZALAY J.-P., OLIVE J.-F., HURLEY K., LEVINE A., MARTEL F., MORGAN E., WOOSLEY S.E., CLINE T., BRAGA J., MANCHANDA R., PIZZICHINI G.
	Astrophys. J., 621, 884-893 (2005)
	High-energy observations of XRF 030723: evidence for an off-axis γ-ray burst?
o	Fig.6, Table 4: <[BSS2005] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSS2007]
[BSS2007]	(Bolatto+Simon+Stanimirovoc+, 2007)= ([BSS2007a])
Write:	<<[BSS2007] NNN>>
N:	282
Object:	Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Stat:	is completely incorporated in Simbad
Note:	Spitzer Survey of the SMC. See also S3MC.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2007ApJ...655..212B
by	BOLATTO A.D. , SIMON J.D., STANIMIROVIC S., VAN LOON J.T., SHAH R.Y., VENN K., LEROY A.K., SANDSTROM K., JACKSON J.M., ISRAEL F.P., LI A., STAVELEY-SMITH L., BOT C., BOULANGER F., RUBIO M.
	Astrophys. J., 655, 212-232 (2007)
	The Spitzer Survey of the Small Magellanic Cloud: S^{3}MC imaging and photometry in the mid- and far-infrared wave bands.
o	Table 4, col.(1): <[BSS2007] NNN> (Nos 1-282) = <S3MC JHHMMSS.ss+DDMMSS.ss> N=282.
=E=	Catalogue in electronic form as J/ApJ/655/212
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSS2007a]
[BSS2007a]	(Bolatto+Simon+Stanimirovoc+, 2007)
*****	Avoid the usage of [BSS2007a], prefer [BSS2007]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSS2007b]
[BSS2007b]	(Bosler+Smecker-Hane+Stetson, 2007)
Write:	<<[BSS2007b] Leo I NNNNN>> <<[BSS2007b] Leo II NNN>>
N:	101+74
Object:	* (SIMBAD class: Star)
Note:	Keck LRIS observations of RGB stars in Leo I and Leo II.
in source:	Leo I = UGC 5470
in source:	Leo II = UGC 6253
Ref:	=2007MNRAS.378..318B
by	BOSLER T.L. , SMECKER-HANE T.A., STETSON P.B.
	Mon. Not. R. Astron. Soc., 378, 318-338 (2007)
	The chemical abundances of the stellar populations in the Leo I and II dSph galaxies.
o	Tables 6, 8: <[BSS2007b] Leo I NNNNN> N=101 among (Nos 2195-25820). Tables 7, 9: <[BSS2007b] Leo II NNN> N=74 among (Nos 156-623).
=E=	Catalogue in electronic form as J/MNRAS/378/318
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BST
BST	(Bingelli+Sandage+Tammann)
*****	Avoid the usage of BST, prefer VCC
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BST93]
[BST93]	(Boroson+Salzer+Trotter, 1993)
Write:	<<[BST93] aF.NNNN>> <<[BST93] aFa.NNNN>>
N:	47
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	In the format, the first letter is always the letter 'a', 'F' and 'Fa' are for fields 1, 3, 4, 6, 8, 9 and 9a, 'NNNN' is a running number in each field.
Ref:	=1993ApJ...412..524B
by	BOROSON T.A. , SALZER J.J., TROTTER A.
	Astrophys. J., 412, 524-534 (1993)
	A new survey for low-luminosity emission-line galaxies.
o	Tables 2,3,4: <[BST93] aFa.NNNN> N=47
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSV2000]
[BSV2000]	(Bicknell+Sutherland+Van Breugel+, 2000) (Not yet in Simbad)
Write:	<<[BSV2000] 4C 41.17 BN>> <<[BSV2000] 4C 41.17 WWW>>
N:	3+4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
in source:	4C 41.17
Ref:	=2000ApJ...540..678B
by	BICKNELL G.V. , SUTHERLAND R.S., VAN BREUGEL W.J.M., DOPITA M.A., DEY A., MILEY G.K.
	Astrophys. J., 540, 678-686 (2000)
	Jet-induced emission-line nebulosity and star formation in the high-redshift radio galaxy 4C 41.17.
o	Fig.1: objects are first cited in Van Breugel+, 1998, 'The most distant radio galaxies, Ed. P. Best+, Dordrecht, Reidel
o	Table 1, Fig.1: <[BSV2000] 4C 41.47 BN> (Nos B1-B3), <[BSV2000] 4C 41.47 WWW> (Nos S, NE, NW, NEE).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSV2011]
[BSV2011]	(Brodwin+Stern+Vikhlinin+, 2011)
Write:	<<[BSV2011] JHHMMSS.s+DDMMSS>>
N:	17+8
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck DEIMOS/LRIS and HST WFC3 grism spectroscopy of N=17+8 galaxies the galaxy clusters ISCS J1438.1+3414 and ISCS J1432.4+3250.
in source:	ISCS J1438.0+3414
in source:	ISCS J1432.0+3250
Ref:	=2011ApJ...732...33B
by	BRODWIN M. , STERN D., VIKHLININ A., STANFORD S.A., GONZALEZ A.H., EISENHARDT P.R., ASHBY M.L.N., BAUTZ M., DEY A., FORMAN W.R., GETTINGS D., HICKOX R.C., JANNUZI B.T., JONES C., MANCONE C., MILLER E.D., MOUSTAKAS L.A., RUEL J., SNYDER G., ZEIMANN G.
	Astrophys. J., 732, 33 (2011)
	X-ray emission from two infrared-selected galaxy clusters at z > 1.4 in the IRAC shallow cluster survey.
o	Table 1: <[BSV2011] JHHMMSS.s+DDMMSS> N=17+8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSW2004]
[BSW2004]	(Beuther+Schilke+Wyrowski, 2004)
Write:	<<[BSW2004] IRAS 20293+3952 mm Na>> <<[BSW2004] IRAS 19410+2336 CS N>>
N:	4+9
Object:	(mm) + Part of Cloud (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	Plateau de Bure Interferometer observations of two star-forming regions IRAS 20293+3952 and IRAS 19410+2336. Millimeter continuum sources are observed in IRAS 20293+3952, and CS features in IRAS 19410+2336 (see also [BSS2003]).
in source:	IRAS 20293+3952
in source:	IRAS 19410+2336
Ref:	=2004ApJ...615..832B
by	BEUTHER H. , SCHILKE P., WYROWSKI F.
	Astrophys. J., 615, 832-839 (2004)
	High spatial resolution CN and CS observation of two regions of massive star formation.
o	Fig.1, Table 2: <[BSW2004] IRAS 20293+3952 mm Na> (Nos 1-3, 1a). Fig.7: <[BSW2004] IRAS 19410+2336 CS N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSW2011]
[BSW2011]	(Bagchi+Sirothia+Werner+, 2011) (Not yet in Simbad)
Write:	<<[BSW2011] RW>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	N=2 radio relics in the galaxy cluster PLCKESZ G287.0+32.9. Use of GMRT (150MHz) and VLA (1.4GHz) data.
in source:	PLCKESZ G287.0+32.9
Ref:	=2011ApJ...736L...8B
by	BAGCHI J. , SIROTHIA S.K., WERNER N., PANDGE M.B., KANTHARIA N.G., ISHWARA-CHANDRA C.H., GOPAL-KRISHNA, PAUL S., JOSHI S.
	Astrophys. J., 736L, 8 (2011)
	Discovery of the first giant double radio relic in a galaxy cluster found in the planck Sunyaev-Zel'dovich cluster survey: PLCK G287.0+32.9.
o	Figs 2-3: <[BSW2011] RW> (Nos RN, RS).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BSZ2018]
[BSZ2018]	(Bennet+Sand+Zaritsky+, 2018)
Write:	<<[BSZ2018] NGC NNNN-Dw1>>
N:	2
Object:	Ultra-diffuse G (SIMBAD class: LowSurfBrghtG = Low Surface Brightness Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Identification of N=2 ultra-diffuse galaxies (UDGs) in the fields of NGC 2708 and NGC 5631. Use of CFHTLS images in the Wide portion.
Ref:	=2018ApJ...866L..11B
by	BENNET P. , SAND D.J., ZARITSKY D., CRNOJEVIC D., SPEKKENS K., KARUNAKARAN A.
	Astrophys. J., 866L, 11-11 (2018)
	Evidence for ultra-diffuse galaxy "formation" through galaxy interactions.
o	Table 1: <[BSZ2018] NGC 2708-Dw1> and <[BSZ2018] NGC 5631-Dw1>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BT2001]
[BT2001]	(Brogan+Troland, 2001) (Not yet in Simbad)
Write:	<<[BT2001] B-17W>> <<[BT2001] B-20UC1>> <<[BT2001] B-20HI>>
N:	3+1+1
Object:	OH condensation (SIMBAD class: Cloud)
Note:	Main OH column density condensations toward M 17.
Ref:	=2001ApJ...560..821B
by	BROGAN C.L. , TROLAND T.H.
	Astrophys. J., 560, 821-840 (2001)
	VLA H I and OH Zeeman observations toward M17.
o	Fig.6, Table 2: <[BT2001] B-17W> (Nos N, C, S), <[BT2001] B-20UC1> N=1, <[BT2001] B-20HI> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BT2003]
[BT2003]	(Bohigas+Tapia, 2003)= ([BT2003a])
Write:	<<[BT2003] NN>> <<[BT2003] AN>>
N:	54
Object:	(Near IR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Stat:	is completely incorporated in Simbad
Note:	OAN observations at San Pedro Martir. Near IR observations of the region Sh 2-128.
in source:	SH 2-128
Ref:	=2003AJ....126.1861B
by	BOHIGAS J. , TAPIA M.
	Astron. J., 126, 1861-1870 (2003)
	Sh 2-128: an H II and star-forming region in the galactic outback.
o	Table 4: <[BT2003] NN> (Nos 1-54), <[BT2003] AN> (Nos N0-N3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BT2003a]
[BT2003a]	(Bohigas+Tapia, 2003)
*****	Avoid the usage of [BT2003a], prefer [BT2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BT2003b]
[BT2003b]	(Boles+Trondal, 2003)
Write:	<<[BT2003b] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Stat:	is completely incorporated in Simbad
Note:	Discovery of a new UK nova (Supernova Patrol) in M 31.
in source:	M 31 = NGC 224
Ref:	=2003IAUC.8205....2B
by	BOLES T. , TRONDAL O.
	IAU Circ., 8205, 2-None (2003)
	Nova in M31.
o	<[BT2003b] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BT2009]
[BT2009]	(Butler+Tan, 2009)
Write:	<<[BT2009] A>> <<[BT2009] ANN>>
N:	10+74
Object:	Dark Cloud + Core (SIMBAD class: DarkNeb = Dark Cloud (nebula))
Note:	MIR extinction mapping of infrared dark clouds using Spitzer GLIMPSE images.
Ref:	=2009ApJ...696..484B
by	BUTLER M.J. , TAN J.C.
	Astrophys. J., 696, 484-497 (2009)
	Mid-infrared extinction mapping of infrared dark clouds: probing the initial conditions for massive stars and star clusters.
o	Table 1: <[BT2009] A> (Nos A-J). Table 3: <[BT2009] ANN> N=74.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BT80]
[BT80]	(Blitz+Thaddeus, 1980)
Write:	<<[BT80] A>> <<[BT80] AN>> <<[BT80] AN-N>>
N:	10+15+15
Object:	Cloud + Part of Cloud (SIMBAD class: MolCld = Molecular Cloud)
Note:	Search for CO clouds in the Assoc. Mon OB 2 in Rosette Molecular Complex, sub-clouds and peaks.
in source:	NAME Rosette Molecular Cloud
Ref:	=1980ApJ...241..676B
by	BLITZ L. , THADDEUS P.
	Astrophys. J., 241, 676-696 (1980)
	Giant molecular complexes and OB associations. I. The Rosette molecular complex.
o	Table 2A: <[BT80] A> (Nos A-J). Table 2B: <[BT80] AN> N=15, <[BT80] AN-N> N=15.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BT97]
[BT97]	(Belloni+Tagliaferri, 1997)
Write:	<<[BT97] NN>>
N:	18
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations.
in source:	NGC 6940
Ref:	=1997A&A...326..608B
by	BELLONI T. , TAGLIAFERRI G.
	Astron. Astrophys., 326, 608-613 (1997)
	Soft X-ray emission from intermediate-age open clusters: NGC 6940.
o	Table 1: <[BT97] NN> (Nos 1-18)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTA2009]
[BTA2009]	(Bradac+Treu+Applegate+, 2009)
Write:	<<[BTA2009] DDD.ddddd+DD.dddddd>>
N:	24
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations of galaxies behind the Bullet cluster.
Ref:	=2009ApJ...706.1201B
by	BRADAC M. , TREU T., APPLEGATE D., GONZALEZ A.H., CLOWE D., FORMAN W., JONES C., MARSHALL P., SCHNEIDER P., ZARITSKY D.
	Astrophys. J., 706, 1201-1212 (2009)
	Focusing cosmic telescopes: exploring redshift z ~ 5-6 galaxies with the bullet cluster 1E0657-56.
o	Table 1: <[BCG2006] A> (Nos K-L) added, <[BCG2006] A DDD.ddddd+DD.ddddd> N=6 added. Table 2: <[BTA2009] DDD.ddddd+DD.ddddd> N=24.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BTA91
BTA91	(Bruhweiler+Truong+Altner, 1991)
Write:	<<BTA91 Na>>
N:	10
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
Note:	IUE observations of NGC 1068: N=10 prominent UV starburst knots (Nos 1-7, 8a-8b, 9)
in source:	NGC 1068
Ref:	=1991ApJ...379..596B
by	BRUHWEILER F.C. , TRUONG K.Q., ALTNER B.
	Astrophys. J., 379, 596-608 (1991)
	IUE observations of NGC 1068 : the extremely luminous starburst knots.
o	Fig.1: <BTA91 Na> (Nos 1-7, 8a-8b, 9).
Origin	of the Acronym: L (1994ApJ...430..545N)
Details on Acronym: [BTB2000]
[BTB2000]	(Buta+Treuthardt+Byrd+, 2000) (Not yet in Simbad)
Write:	<<[BTB2000] NNN>>
N:	25
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
in source:	NGC 1326
Ref:	=2000AJ....120.1289B
by	BUTA R. , TREUTHARDT P.M., BYRD G.G., CROCKER D.A.
	Astron. J., 120, 1289-1305 (2000)
	Circumnuclear star formation in the early-type resonance ring barred spiral galaxy NGC 1326.
o	(Erratum) Erratum vol.122 p.2785 (2000)
o	Table 1: <[BTB2000] NNN> N=25 among (Nos 1-803).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BTC
BTC	(Big Throughput Camera)
*****	Avoid the usage of BTC, prefer [HHG2004]
Origin	of the Acronym: L (2008ApJ...682..199W)
Details on Acronym: BTC
BTC	(Big Throughput Camera)
*****	Avoid the usage of BTC, prefer [THM2001]
Origin	of the Acronym: L (2005A&A...440...61R)
Details on Acronym: [BTC2001]
[BTC2001]	(Butt+Torres+Combi+, 2001)
Write:	<<[BTC2001] Cloud A>>
N:	3
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	N=3 massive and dense molecular clouds lying adjacent to the SNR RX J1713.7-3946. See also [SGD99].
Ref:	=2001ApJ...562L.167B
by	BUTT Y.M. , TORRES D.F., COMBI J.A., DAME T., ROMERO G.E.
	Astrophys. J., 562, 167-171 (2001)
	Is the supernova remnant RX J1713.7-3946 a hadronic cosmic-ray accelerator.
o	Fig.1: <[BTC2001] Cloud A> (Nos A-B).
Ref:	=2003A&A...400..567U
by	UCHIYAMA Y. , AHARONIAN F.A., TAKAHASHI T.
	Astron. Astrophys., 400, 567-574 (2003)
	Fine-structure in the nonthermal X-ray emission of SNR RX J1713.7-3946 revealed by Chandra.
o	Fig.1: <[BTC2001] Cloud A> (No. C) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTC2018]
[BTC2018]	(Beck+Turner+Consiglio, 2018)
Write:	<<[BTC2018] NN>>
N:	71
Object:	Molecular Clump (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	ALMA CO(3-2) observations of N=71 molecular clumps in the dwarf galaxy Henize 2-10.
in source:	Hen 2-10
Ref:	=2018ApJ...867..165B
by	BECK S.C. , TURNER J.L., CONSIGLIO S.M.
	Astrophys. J., 867, 165-165 (2018)
	Dense molecular filaments feeding a starburst: ALMA maps of co(3-2) in Henize 2-10.
o	<NAME Henize 2-10 Bird> N=1. Table 2: <[BTC2018] NN> (Nos 0-70).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BTC40
BTC40	(Big Throughput Camera, 40deg2 survey)
Write:	<<BTC40 JHHMM+DDMM>>
N:	40
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Note:	BTC40 survey on the CTIO 4m telescope to search for QSOs of 4.8<z<6.
Ref:	=2002AJ....124.2971M
by	MONIER E.M. , KENNEFICK J.D., HALL P.B., OSMER P.S., SMITH M.G., DALTON G.B., GREEN R.F.
	Astron. J., 124, 2971-2979 (2002)
	The BTC40 survey for quasars at 4.8<z<6.
o	Table 4, object 3 = BTC40 J0001-4024 not 4025. Table 4, col(1): numbering NN not in SIMBAD.
o	Table 2: <BTC40 JHHMM+DDMM> N=40.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BTG2001]
[BTG2001]	(Beck+Turner+Gorjian, 2001) (Not yet in Simbad)
Write:	<<[BTG2001] A>>
N:	3
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
in source:	Hen 2-10
Ref:	=2001AJ....122.1365B
by	BECK S.C. , TURNER J.L., GORJIAN V.
	Astron. J., 122, 1365-1368 (2001)
	Infrared emission from clusters in the star-forming disk of Henize 2-10.
o	Table 1: <[BTG2001] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTG2004]
[BTG2004]	(Baker+Tacconi+Genzel+, 2004)
Write:	<<[BTG2004] X>>
N:	1
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	IRAM PdB observations of cB58 (NAME cB58 in SIMBAD). Discovery of an additional 'X' source in the field of cB58.
Ref:	=2004ApJ...604..125B
by	BAKER A.J. , TACCONI L.J., GENZEL R., LEHNERT M.D., LUTZ D.
	Astrophys. J., 604, 125-140 (2004)
	Molecular gas in the lensed Lyman break galaxy cB58.
o	Table 1: PPP NNNNNN = CNOC MS 1512 NNNNNN in S. Parag. 4.1: Westphal-MD11 = Westphal MMD11 in S.
o	Table 1: <[BTG2004] A> (No. X).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTG98]
[BTG98]	(Bock+Turtle+Green, 1998)
Write:	<<[BTG98] N>>
N:	5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	(Nos 1-3) are filaments in the field of Vela SNR, (Nos 4-5) are objects in the same field.
Ref:	=1998AJ....116.1886B
by	BOCK D.C.-J. , TURTLE A.J., GREEN A.J.
	Astron. J., 116, 1886-1896 (1998)
	A high-resolution radio survey of the Vela supernova remnant.
o	Fig.5: <[BTG98] N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTH2006]
[BTH2006]	(Battaglia+Tolstoy+Helmi+, 2006)
Write:	<<[BTH2006] fnx-NN NNN>> <<[BTH2006] ETNNN>>
N:	383+257
Object:	* (SIMBAD class: Star)
Note:	ESO WFI2.2m and VLT FLAMES observations of the Fornax Dwarf Galaxy.
in source:	NAME Fornax Dwarf Galaxy
Ref:	=2006A&A...459..423B
by	BATTAGLIA G. , TOLSTOY E., HELMI A., IRWIN M.J., LETARTE B., JABLONKA P., HILL V., VENN K.A., SHETRONE M.D., ARIMOTO N., PRIMAS F., KAUFER A., FRANCOIS P., SZEIFERT T., ABEL T., SADAKANE K.
	Astron. Astrophys., 459, 423-440 (2006)
	The DART imaging and CaT survey of the Fornax dwarf spheroidal galaxy.
o	Table 4: <[BTH2006] fnx-NN NNN> N=383, <[BTH2006] ETNNN> N=257 among (Nos 007-327).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTH2011]
[BTH2011]	(Battaglia+Tolstoy+Helmi+, 2011)
Write:	<<[BTH2011] NNN>>
N:	174
Object:	RGB* (SIMBAD class: RGB* = Red Giant Branch star)
Stat:	is completely incorporated in Simbad
Note:	VLT FLAMES observations of N=174 RGB stars that are probable members of the Sextans dwarf spheroidal galaxy.
in source:	NAME Sextans Dwarf Galaxy
Ref:	=2011MNRAS.411.1013B
by	BATTAGLIA G. , TOLSTOY E., HELMI A., IRWIN M., PARISI P., HILL V., JABLONKA P.
	Mon. Not. R. Astron. Soc., 411, 1013-1034 (2011)
	Study of the Sextans dwarf spheroidal galaxy from the DART Ca II triplet survey.
o	Table 3: <[BTH2011] NNN> (Nos 1-174).
=E=	Catalogue in electronic form as <J/MNRAS/411/1013/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTI2004]
[BTI2004]	(Bouwens+Thompson+Illingworth+, 2004)= (UDF)
Write:	<<[BTI2004] UDF-NNN-NNNN>>
N:	6
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	NICMOS observations of the HUDF.
in source:	NAME HUDF
Ref:	=2004ApJ...616L..79B
by	BOUWENS R.J. , THOMPSON R.I., ILLINGWORTH G.D., FRANX M., VAN DOKKUM P.G., FAN X., DICKINSON M.E., EISENSTEIN D.J., RIEKE M.J.
	Astrophys. J., 616, 79-82 (2004)
	Galaxies at z~7-8: z_{850}-Dropouts in the Hubble Ultra Deep Field.
o	Table 1: <[BTI2004] UDF-NNN-NNNN> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTK2000]
[BTK2000]	(Beck+Turner+Kovo, 2000)
Write:	<<[BTK2000] NGC 4214 WN>> <<[BTK2000] Mrk 8 A>> <<[BTK2000] Tol 35 A>> <<[BTK2000] Mrk 1236 A>> <<[BTK2000] Pox 4 A>>
N:	6+4+2+2+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Radio-sources or clumps in 5 Wolf-Rayet galaxies.
in source:	NGC 4214
in source:	Mrk 8
in source:	Tol 35
in source:	Mrk 1236
in source:	POX 4
Ref:	=2000AJ....120..244B
by	BECK S.C. , TURNER J.L., KOVO O.
	Astron. J., 120, 244-259 (2000)
	High-resolution radio maps of Wolf-Rayet galaxies: optically thick H II regions?
o	T.3: Mrk 1089A and B = [CLV96] NGC 1741 A and B.
o	Table 3, 4: <[BTK2000] NGC 4214 WN> (Nos N, S, N1-N2, S1-S2), <[BTK2000] Mrk 8 A> (Nos A-D), <[BTK2000] Tol 35 A> (Nos A-B), <[BTK2000] Mrk 1236 A> (Nos A-B), <[BTK2000] Pox 4 A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTK2009]
[BTK2009]	(Bastian+Trancho+Konstantopoulos+, 2009)
Write:	<<[BTK2009] TNNN>>
N:	16
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Gemini North telescope GMOS observations of the Antennae. Use of HST images.
in source:	NAME the Antennae
Ref:	=2009ApJ...701..607B
by	BASTIAN N. , TRANCHO G., KONSTANTOPOULOS I.S., MILLER B.W.
	Astrophys. J., 701, 607-619 (2009)
	Gemini spectroscopic survey of young star clusters in Merging/Interacting galaxies. III. The Antennae.
o	Tables 1-3, Fig. 1: <[BTK2009] TNNN> N=16 among (Nos 54-395).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTK93]
[BTK93]	(Bernstein+Tyson+Kochanek, 1993)
Write:	<<[BTK93] AN>>
N:	2
Object:	Arc (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Stat:	is completely incorporated in Simbad
Note:	In the field of the lensed QSO 0957+561, the most striking feature is an arc, divided into 2 parts A1 and A2 (Map Plate 38) See also YGKOW, [RGH85], [GWC92], [ACL97], [BFT97], [BLF99], [PMN99], [SOS99], [TF99].
in source:	QSO B0957+561
Ref:	=1993AJ....105..816B
by	BERNSTEIN G.M. , TYSON J.A., KOCHANEK C.S.
	Astron. J., 105, 816-830 (1993)
	A large arc in the gravitational lens system 0957+561.
o	Text and fig.1: galaxies G1, G5 = YGKOW G1, G5. P.820: sources A to E = [RGH85] A to E.
o	Table 1: <[BTK93] AN> (Nos A1-A2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTK98]
[BTK98]	(Bershady+Trevese+Kron, 1998)= (N2540)
Write:	<<[BTK98] NNNN>>
N:	16
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Note:	Table 3: N=16 objects from the 'N2540' Rome catalog (designation used by the authors) See also T89 and [MKK97]
in source:	SA 57-
Ref:	=1998ApJ...496..103B
by	BERSHADY M.A. , TREVESE D., KRON R.G.
	Astrophys. J., 496, 103-116 (1998)
	Variable extended objects in selected area 57.
o	Table 3: NSer = [MKK97]
o	Table 3: <[BTK98] NNNN> N=16 among 2540
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTL2000]
[BTL2000]	(Becker+Trumper+Lommen+, 2000)
Write:	<<[BTL2000] NN>>
N:	17
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations of PSR J0030+0451 field.
Ref:	=2000ApJ...545.1015B
by	BECKER W. , TRUMPER J., LOMMEN A.N., BACKER D.C.
	Astrophys. J., 545, 1015-1019 (2000)
	X-rays from the nearby solitary millisecond pulsar PSR J0030+0451: the final ROSAT observations.
o	Table 1: <[BTL2000] NN> (Nos 1-17).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTL2002]
[BTL2002]	(Beck+Turner+Langland-Shula+, 2002) (Not yet in Simbad)
Write:	<<[BTL2002] JHHMMSS.sss+DDMMSS.ss>>
N:	5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA observations of the starburst galaxy Zw II 40.
in source:	ZW II 40
Ref:	=2002AJ....124.2516B
by	BECK S.C. , TURNER J.L., LANGLAND-SHULA L.E., MEIER D.S., CROSTHWAITE L.P., GORJIAN V.
	Astron. J., 124, 2516-2523 (2002)
	Radio-infrared supernebulae in II Zw 40.
o	Figs 1+4, Text: <[BTL2002] JHHMMSS.sss+DDMMSS.ss> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTM2020]
[BTM2020]	(Bruzzese+Thilker+Meurer+, 2020)
Write:	<<[BTM2020] HII-N>>
N:	6
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	HST ACS/WFC observations of N=6 HII regions in the outer disk of M83.
in source:	NGC 5236 = M 83
Ref:	=2020MNRAS.491.2366B
by	BRUZZESE S.M. , THILKER D.A., MEURER G.R., BIANCHI L., WATTS A.B., FERGUSON A.M.N., GIL DE PAZ A., MADORE B., MARTIN D.C., RICH R.M.
	Mon. Not. R. Astron. Soc., 491, 2366-2390 (2020)
	The initial mass function in the extended ultraviolet disc of M83.
o	Fig. 7, Table 4: <[BTM2020] HII-N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTM97]
[BTM97]	(Blakeslee+Tonry+Metzger, 1997)
Write:	<<[BTM97] ACO NNNN N>>
N:	23
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=23 Brightest Cluster Galaxies (BCG) in 19 ACO clusters
Ref:	=1997AJ....114..482B
by	BLAKESLEE J.P. , TONRY J.L., METZGER M.R.
	Astron. J., 114, 482-506 (1997)
	Globular clusters in 19 northern Abell clusters.
o	Table 1: <[BTM97] ACO NNNN N> N=23
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTP2019]
[BTP2019]	(Burchett+Tripp+Prochaska+, 2019)
Write:	<<[BTP2019] JHHMM+DDMM NNN NN>> <<[BTP2019] JHHMM+DDMM_NNN_NN>> (not recognised by Simbad, but found in literature)
N:	29
Object:	G (SIMBAD class: Galaxy)
Note:	HST COS and STIS observations of N=24 galaxies at 0.49<z_gal<1.44. Use of data from the COS Absorption Survey of Baryon Harbors (CASBaH).
Ref:	=2019ApJ...877L..20B
by	BURCHETT J.N. , TRIPP T.M., PROCHASKA J.X., WERK J.K., TUMLINSON J., HOWK J.C., WILLMER C.N.A., LEHNER N., MEIRING J.D., BOWEN D.V., BORDOLOI R., PEEPLES M.S., JENKINS E.B., O'MEARA J.M., TEJOS N., KATZ N.
	Astrophys. J., 877L, 20-20 (2019)
	The COS Absorption Survey of Baryon Harbors (CASBaH): warm-hot circumgalactic gas reservoirs traced by Ne VIII Absorption.
o	Table 1: <[BTP2019] JHHMM+DDMM_{NNN}NN> N=29.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTR2004]
[BTR2004]	(Bohigas+Tapia+Roth+, 2004)
Write:	<<[BTR2004] NN>>
N:	26
Object:	(Near IR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Stat:	is completely incorporated in Simbad
Note:	N=26 sources with Near-IR excess, embedded in the HII region Gal 353.2+0.9. Use of 2MASS archival data.
in source:	GAL 353.2+00.9
Ref:	=2004AJ....127.2826B
by	BOHIGAS J. , TAPIA M., ROTH M., RUIZ M.T.
	Astron. J., 127, 2826-2837 (2004)
	Optical imaging and spectroscopy of the H II region G353.2+0.9 in NGC 6357 and its relation to Pismis 24.
o	Table 5: <[BTR2004] NN> (Nos 1-26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTR99]
[BTR99]	(Beuermann+Thomas+Reinsch+, 1999)
Write:	<<[BTR99] JHHMMSS.s+DDMMSS>>
N:	74
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 3: Counterpart of RX sources. 1RXS J013653.5-351012 has 2 possible counterparts, 1RXS J061544.4-653151 has 3 possible counterparts.
Ref:	=1999A&A...347...47B
by	BEUERMANN K. , THOMAS H.-C., REINSCH K., SCHWOPE A.D., TRUEMPER J., VOGES W.
	Astron. Astrophys., 347, 47-54 (1999)
	Identification of soft high galactic latitude RASS X-ray sources. II. Sources with PSPC count rate CR <0.5cts/s.
o	Table 3: <[BTR99] JHHMMSS.s+DDMMSS> N=74.
=E=	Catalogue in electronic form as J/A+A/347/47
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BTS
BTS	(Binggeli+Tarenghi+Sandage)
Write:	<<BTS NNN>>
N:	179
Object:	Dwarf G (SIMBAD class: Galaxy)
Note:	(Nos 1-179), dwarf and dwarf candidate galaxies in the field defined as the space outside of rich clusters of galaxies.
Ref:	=1990A&A...228...42B
by	BINGGELI B. , TARENGHI M., SANDAGE A.
	Astron. Astrophys., 228, 42-60 (1990)
	The abundance and morphological segregation of dwarf galaxies in the field.
o	Table 2: <BTS NNN> (Nos 1-179)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BTS2010]
[BTS2010]	(Bridge+Teplitz+Siana+, 2010)
Write:	<<[BTS2010] C-UVLG-NN>>
N:	32
Object:	G (SIMBAD class: Galaxy)
Note:	HST ACS/SBC UV spectroscopy and Palomar Hale 5-m telescope optical spectroscopy of N=32 UV luminous galaxies (UVLG). Use of GALEX photometry, HST F814W imaging and zCOSMOS data.
in source:	NAME COSMOS Field
Ref:	=2010ApJ...720..465B
by	BRIDGE C.R. , TEPLITZ H.I., SIANA B., SCARLATA C., CONSELICE C.J., FERGUSON H.C., BROWN T.M., SALVATO M., RUDIE G.C., DE MELLO D.F., COLBERT J., GARDNER J.P., GIAVALISCO M., ARMUS L.
	Astrophys. J., 720, 465-479 (2010)
	A spectroscopic search for leaking Lyman continuum at z ~ 0.7.
o	Fig. 2, Table 1: <[BTS2010] C-UVLG-NN> N=32 among (Nos 2-35).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTS2017]
[BTS2017]	(Bauer+Treister+Schawinski+, 2017)
Write:	<<[BTS2017] CDF-S XTN>>
N:	2
Object:	X-ray Transient (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-I observations of N=2 fast X-ray transients in the Chandra Deep Field South.
in source:	NAME CDFS
Ref:	=2017MNRAS.467.4841B
by	BAUER F.E. , TREISTER E., SCHAWINSKI K., SCHULZE S., LUO B., ALEXANDER D.M., BRANDT W.N., COMASTRI A., FORSTER F., GILLI R., KANN D.A., MAEDA K., NOMOTO K., PAOLILLO M., RANALLI P., SCHNEIDER D.P., SHEMMER O., TANAKA M., TOLSTOV A., TOMINAGA N., TOZZI P., VIGNALI C., WANG J., XUE Y., YANG G.
	Mon. Not. R. Astron. Soc., 467, 4841-4857 (2017)
	A new, faint population of X-ray transients.
o	<[BTS2017] CDF-S XTN> (No. XT1).
Ref:	=2019Natur.568..198X
by	XUE Y.Q. , ZHENG X.C., LI Y., BRANDT W.N., ZHANG B., LUO B., ZHANG B.-B., BAUER F.E., SUN H., LEHMER B.D., WU X.-F., YANG G., KONG X., LI J.Y., SUN M.Y., WANG J.-X., VITO F.
	Natur, 568, 198-201 (2019)
	A magnetar-powered X-ray transient as the aftermath of a binary neutron-star merger.
o	<[BTS2017] CDF-S XTN> (No. XT2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BTS87
BTS87	(Binggeli+Tammann+Sandage)
Write:	<<BTS87 Cluster A>> <<BTS87 Cloud A>> <<BTS87 Cloud A'>>
N:	5
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=5 groups of galaxies in Virgo cluster, Cluster A (NGC 4486 or M 87 group) and Cluster B (NGC 4472 or M 49 group), Cloud W and Cloud W' already found in De Vaucouleurs [D61], Cloud M already found in Ftaclas+ [FFS84].
in source:	NAME Virgo Cluster
Ref:	=1987AJ.....94..251B
by	BINGGELI B. , TAMMANN G.A., SANDAGE A.
	Astron. J., 94, 251-277 (1987)
	Studies of the Virgo cluster. VI. Morphological and kinematical structure of the Virgo cluster.
o	<BTS87 Cluster A>, <BTS87 Cluster B>, <BTS87 Cloud W>, <BTS87 Cloud W'>, <BTS87 Cloud M>
Origin	of the Acronym: L (1993A&AS...98..275B)
Details on Acronym: [BTT2002]
[BTT2002]	(Bosch+Terlevich+Terlevich, 2002)
Write:	<<[BTT2002] NGC 5447 A>> <<[BTT2002] NGC 5462 A>>
N:	3+5
Object:	? (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	JKT La Palma observations. Knots in HII regions NGC 5447 and NGC 5462.
in source:	NGC 5447
in source:	NGC 5462
Ref:	=2002MNRAS.329..481B
by	BOSCH G. , TERLEVICH E., TERLEVICH R.
	Mon. Not. R. Astron. Soc., 329, 481-496 (2002)
	Narrow-band CCD photometry of giant H II regions.
o	Fig.23: [MGC95] NGC 5461 A to E. Fig.25: [S85b] A to E, A'.
o	Fig.22: <[BTT2002] NGC 5447 A> (Nos A-C). Fig.24: <[BTT2002] NGC 5462 A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTW2002]
[BTW2002]	(Becker+Tyson+Wittman+, 2002)
Write:	<<[BTW2002] JHHMMSS.ss+DDMMSS.s>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxies of SN 2002AJ, SN 2002AL, and SN 2002AM.
Ref:	=2002IAUC.7804....1B
by	BECKER A. , TYSON T., WITTMAN D., LOPEZ-CANIEGO M., NORMAN D., CLOCCHIATTI A., DELL'ANTONIO I., SQUIRES G., (The Deep Lens Survey Team)
	IAU Circ., 7804, 1-None (2002)
	Supernovae 2002aj, 2002ak, 2002al, 2002am.
o	Host galaxy of SN 2002AK is not defined.
o	<[BTW2002] JHHMMSS.ss+DDMMSS.s> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTW2003]
[BTW2003]	(Braun+Thilker+Walterbos, 2003)
Write:	<<[BTW2003] JHHMM+DDMM>>
N:	146
Object:	HI G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Search for HI detected galaxies with the Westerbock array.
Ref:	=2003A&A...406..829B
by	BRAUN R. , THILKER D., WALTERBOS R.A.M.
	Astron. Astrophys., 406, 829-846 (2003)
	The WSRT wide-field HI survey. I. The background galaxy sample.
o	Table 1: <[BTW2003] JHHMM+DDMM> N=146.
=E=	Catalogue in electronic form as J/A+A/406/829
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTW2010]
[BTW2010]	(Bennert+Treu+Woo+, 2010)
Write:	<<[BTW2010] SSNN>>
N:	16
Object:	Seyfert-1 G (SIMBAD class: Seyfert1 = Seyfert 1 Galaxy)
Note:	HST NICMOS observations of Seyvert-1 galaxies. See also [TMB2004], [WTM2008].
Ref:	=2010ApJ...708.1507B
by	BENNERT V.N. , TREU T., WOO J.-H., MALKAN M.A., LE BRIS A., AUGER M.W., GALLAGHER S., BLANDFORD R.D.
	Astrophys. J., 708, 1507-1527 (2010)
	Cosmic evolution of black holes and spheroids. IV. The M_{BH}–L{sph}Relation.
o	Tables 1-2: <[BTW2010] SSNN> N=13 among (Nos SS1-SS18). Tables 1-2: <[WTM2008] WNN> (Nos W8, W12, W16, W20) added.
Ref:	=2015ApJ...799..164P
by	PARK D. , WOO J.-H., BENNERT V.N., TREU T., AUGER M.W., MALKAN M.A.
	Astrophys. J., 799, 164 (2015)
	Cosmic evolution of black holes and spheroids. V. The relation between black hole mass and host galaxy luminosity for a sample of 79 active galaxies.
o	Table 1: <[BTW2010] SSNN> (Nos SS3, SS4, SS15), <[WTM2008] WNN> (Nos W1-W5, W10, W14, W17) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTW2011]
[BTW2011]	(Buie+Trilling+Wasserman+, 2011) (Not yet in Simbad)
Write:	<<[BTW2011] NNNNNNN+NNNNNN>>
N:	213272
Note:	Lowell Observatory 0.8m and Hall 1.2m telescopes, SMARTS 0.9m telescope, University of Arizona 1.5m Kuiper telescope observations for the calibration of the Deep Ecliptic Survey.
Ref:	=2011ApJS..194...40B
by	BUIE M.W. , TRILLING D.E., WASSERMAN L.H., CRUDO R.A.
	Astrophys. J., Suppl. Ser., 194, 40 (2011)
	A large and faint photometric catalog on the ecliptic.
o	Table 4: <[BTW2011] NNNNNNN+NNNNNN> N=213272.
=E=	Catalogue in electronic form as <J/ApJS/194/40/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTW2018]
[BTW2018]	(Burchett+Tripp+Wang+, 2017)
Write:	<<[BTW2018] JHHMMSS.ss+DDMMSS.ss>> <<[BTW2018] JHHMMSS.s+DDMMSS.ss>> <<[BTW2018] JHHMMSS.ssss+DDMMSS.ssss>> <<[BTW2018] JHHMMSS.ssss+DDMMSS.sss>> <<[BTW2018] JHHMMSS.sss+DDMMSS.ssss>> <<[BTW2018] JHHMMSS.sss+DDMMSS.sss>> <<[BTW2018] JHHMMSS.ssss+DDMMSS.ss>> <<[BTW2018] JHHMMSS.ss+DDMMSS.ssss>> <<[BTW2018] A2246 NN>>
N:	2508+310+347+33+24+3+5+3+17
Object:	G (SIMBAD class: Galaxy)
Note:	MMT Hectospec, and WHT LDSS2 observations of N=2508+310+347+33+24+3+5+3+17 galaxies in the fields of the galaxy clusters ACO 1095, ACO 1926, and ACO 2246. Use of SDSS data.
in source:	ACO 1095
in source:	ACO 1926
in source:	ACO 2246
Ref:	=2018MNRAS.475.2067B
by	BURCHETT J.N. , TRIPP T.M., WANG Q.D., WILLMER C.N.A., BOWEN D.V., JENKINS E.B.
	Mon. Not. R. Astron. Soc., 475, 2067-2085 (2018)
	Warm-hot gas in X-ray bright galaxy clusters and the H I-deficient circumgalactic medium in dense environments.
o	Table A1: <[BTW2018] JHHMMSS.ss+DDMMSS.ss> N=2508, <[BTW2018] JHHMMSS.s+DDMMSS.ss> N=310, <[BTW2018] JHHMMSS.ssss+DDMMSS.ssss> N=347, <[BTW2018] JHHMMSS.ssss+DDMMSS.sss> N=33, <[BTW2018] JHHMMSS.sss+DDMMSS.ssss> N=24, <[BTW2018] JHHMMSS.sss+DDMMSS.sss> N=3, <[BTW2018] JHHMMSS.ssss+DDMMSS.ss> N=5, <[BTW2018] JHHMMSS.ss+DDMMSS.ssss> N=3, <[BTW2018] A2246 NN> (Nos 0-16).
=E=	Catalogue in electronic form as <J/MNRAS/475/2067/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTY2010]
[BTY2010]	(Borthakur+Tripp+Yun+, 2010)
Write:	<<[BTY2010] GQ1042+0747>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Galaxy close (2.5"=1.7kpc) to the QSO (SDSS J104257.58+074850.5). In the format, GQ stands for "galaxy on top of QSO".
Ref:	=2010ApJ...713..131B
by	BORTHAKUR S. , TRIPP T.M., YUN M.S., MOMJIAN E., MEIRING J.D., BOWEN D.V., YORK D.G.
	Astrophys. J., 713, 131-145 (2010)
	Using 21 cm absorption in small impact parameter galaxy-quasar pairs to probe low-redshift damped and sub-damped Lyα systems.
o	Table 1: <[BTY2010] GQ J1042+0747> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTY2011]
[BTY2011]	(Borthakur+Tripp+Yun+, 2011)
Write:	<<[BTY2011] JHHMMSS.ss+DDMMSS.s>>
N:	17
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Apache Point Observatory spectroscopy of N=16 foreground galaxies, in the line of sight of QSOs. Use of archival SDSS data.
Ref:	=2011ApJ...727...52B
by	BORTHAKUR S. , TRIPP T.M., YUN M.S., BOWEN D.V., MEIRING J.D., YORK D.G., MOMJIAN E.
	Astrophys. J., 727, 52 (2011)
	A Green Bank Telescope survey for H I 21 cm absorption in the disks and halos of low-redshift galaxies.
o	Table 1, col(5): <[BTY2011] JHHMMSS.ss+DDMMSS.s> N=17.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BTZ98]
[BTZ98]	(Balaguer-Nunez+Tian+Zhao, 1998)
Write:	<<[BTZ98] NNN>>
N:	722
Object:	* in Cl* (SIMBAD class: Star)
in source:	NGC 1817
in source:	NGC 1807
Ref:	=1998A&AS..133..387B
by	BALAGUER-NUNEZ L. , TIAN K.P., ZHAO J.L.
	Astron. Astrophys., Suppl. Ser., 133, 387-394 (1998)
	Determination of proper motions and membership of the open clusters NGC 1817 and NGC 1807.
o	Table 5: <[BTZ98] NNN> N=722 among (Nos 1-918).
=E=	Catalogue in electronic form as J/A+AS/133/387
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Bu
Bu	(Butler)
Write:	<<Bu LMC I ZNN>> <<Bu LMC II ZNN>> <<Bu SMC ZNN>> <<Bu SMC RNN>> <<Bu SMC M>> <<Bu LMC AN>> <<Bu LMC AANN>> <<Bu SMC AANN>>
N:	63+68+50+23+1+93+115
Object:	* (SIMBAD class: Star)
Note:	Table 5: secondary standards in the LMC I field, format 'LMC I ZNN', (Nos Z1-Z63) Table 6: secondary standards in the LMC II field, format 'LMC II ZNN', (Nos Z1-Z68) Table 7: secondary standards in the SMC, format 'SMC M', N=1, format 'SMC ZNN', (Nos Z1-Z50), format 'SMC RNN', N=23 among (Nos R3-R45) Tables 9, 10: standards in the LMC, format 'LMC AANN' or 'LMC AN', N=93, the letters AA and A stand for sequences OA to OM, and A to N Table 11: standards in the SMC, format 'SMC AANN', N=115, the letters AA stand for sequences OA to OJ
in source:	Magellanic Clouds:LMC = LMC
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1972DunOP...1..133B
by	BUTLER C.J.
	Dunsink Observatory, Dublin, Ireland - Publications, 1, 133-192 (1972)
	Photometric standards in the Magellanic Clouds.
o	Table 5: <Bu LMC I ZNN> (Nos Z1-Z63), Table 6: <Bu LMC II ZNN> (Nos Z1-Z68), Table 7: <Bu SMC M> N=1, <Bu SMC ZNN> (Nos Z1-Z50), <Bu SMC RNN> N=23 among (Nos R3-R45), Table 9, 10: <Bu LMC AANN> and <Bu LMC AN> N=93, Table 11: <Bu SMC AANN> N=115
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Buc
Buc	(Bucarest) (Not yet in Simbad)
Write:	<<Buc NNN>>
N:	212
Object:	V* (SIMBAD class: Variable* = Variable Star)
Rem:	V* Nomenclature.
Details on Acronym: [BUF2019]
[BUF2019]	(Billington+Urquhart+Figura+, 2019)
Write:	<<[BUF2019] GLLL.llll+BB.bbbb>>
N:	44
Object:	Clump (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	ATCA NH3 observations of N=44 clumps in 34 regions identified by the Red MSX Source (RMS) survey.
Ref:	=2019MNRAS.483.3146B
by	BILLINGTON S.J. , URQUHART J.S., FIGURA C., EDEN D.J., MOORE T.J.T.
	Mon. Not. R. Astron. Soc., 483, 3146-3167 (2019)
	The RMS survey: Ammonia mapping of the environment of young massive stellar objects - II.
o	Tables 3-4: <[BUF2019] GLLL.llll+BB.bbbb> N=44.
=E=	Catalogue in electronic form as <J/MNRAS/483/3146/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [BUG2007]
[BUG2007]	(Bresolin+Urbaneja+Gieren+, 2007)
Write:	<<[BUG2007] A NNa>> <<[BUG2007] ANNa>> (not recognised by Simbad, but found in literature)
N:	20+19+18
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 observations of blue supergiant candidates. See also [SK76].
in source:	IC 1613
Ref:	=2007ApJ...671.2028B
by	BRESOLIN F. , URBANEJA M.A., GIEREN W., PIETRZYNSKI G., KUDRITZKI R.-P.
	Astrophys. J., 671, 2028-2039 (2007)
	VLT spectroscopy of blue supergiants in IC 1613.
o	Table 1: <[BUG2007] A NNa> N=20+19+18.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BUN2004]
[BUN2004]	(Bamba+Ueno+Nakajima+, 2004)
Write:	<<[BUN2004] Shell A>> <<[BUN2004] N>>
N:	4+6
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton and Chandra observations around 30 Dor C in the LMC.
in source:	Magellanic Clouds:LMC:30 Dor C = 30 Dor C
Ref:	=2004ApJ...602..257B
by	BAMBA A. , UENO M., NAKAJIMA H., KOYAMA K.
	Astrophys. J., 602, 257-263 (2004)
	Thermal and nonthermal x-rays from the Large Magellanic Cloud superbubble 30 Doradus C.
o	Fig.1: <[BUN2004] Shell A> (Nos A-D). Table 2: <[BUN2004] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Buonanno
Buonanno	(Buonanno+)
*****	Avoid the usage of Buonanno, prefer [BCF85]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BV
BV	(Bohm-Vitense)
Write:	<<BV III-NN>> <<BV V-NN>>
N:	23+21
Object:	Exgl N (SIMBAD class: ISM = Interstellar Medium Object)
Note:	Tables I, II: (Nos 1-23) extragal. neb. in area III, format 'III-NN' Tables III, IV: (Nos 1-21) extragal. neb. in area V, format 'V-NN'
Ref:	=1956PASP...68..430B
by	BOHM-VITENSE E.
	Publ. Astron. Soc. Pac., 68, 430-436 (1956)
	Extragalactic nebulae close to the galactic plane.
o	Tables I,II: <BV III-NN> (Nos 1-23), Tables III,IV: <BV V-NN> (Nos 1-21), Table V: <PN BV N> (Nos 1-3)
Details on Acronym: BV
BV	(Bohm-Vitense)= (BV 5-)
Write:	<<PN BV N>>
N:	3
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Table V
Ref:	=1956PASP...68..430B
by	BOHM-VITENSE E.
	Publ. Astron. Soc. Pac., 68, 430-436 (1956)
	Extragalactic nebulae close to the galactic plane.
o	Tables I,II: <BV III-NN> (Nos 1-23), Tables III,IV: <BV V-NN> (Nos 1-21), Table V: <PN BV N> (Nos 1-3)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BV
BV	(Bamberg, Variable *)
Write:	<<*SV BV** NNNN>>
N:	1641
Object:	V* (SIMBAD class: Variable* = Variable Star)
Rem:	V* Nomenclature.
Details on Acronym: BV 5-
BV 5-	(Bohm-Vitense, Table V)
*****	Avoid the usage of BV 5-, prefer BV
Details on Acronym: [BV92]
[BV92]	(Boulanger+Viallefond, 1992)
Write:	<<[BV92] NN>> <<[BV92] HHMMSS+DDMMSS>>
N:	37+6
Object:	HI (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	Table 4: format 'NN', N=37 HI complexes in NGC 6946 Table 5: format 'HHMMSS+DDMMSS', N=6 HI holes
in source:	NGC 6946
Ref:	=1992A&A...266...37B
by	BOULANGER F. , VIALLEFOND F.
	Astron. Astrophys., 266, 37-56 (1992)
	Observational study of the spiral galaxy NGC 6946. I. HI and radio continuum observations.
o	Table 4: <[BV92] NN> N=37, Table 5: <[BV92] HHMMSS+DDMMSS> N=6
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BV96]
[BV96]	(Belloni+Verbunt, 1996)= (X)
Write:	<<[BV96] NN>>
N:	49
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations
in source:	NGC 752
Ref:	=1996A&A...305..806B
by	BELLONI T. , VERBUNT F.
	Astron. Astrophys., 305, 806-810 (1996)
	Soft X-rays from the intermediate-age open cluster NGC 752.
o	Table 1: <[BV96] NN> (Nos 1-49)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVB2012]
[BVB2012]	(Brogaard+VandenBerg+Bruntt+, 2012)
Write:	<<[BVB2012] NNNNN>>
N:	15395
Object:	* (SIMBAD class: Star)
Note:	Photometric data for N=15395 stars in NGC 6791. Use of NOT observations (see 2003PASP..115..413S).
in source:	NGC 6791
Ref:	=2012A&A...543A.106B
by	BROGAARD K. , VANDENBERG D.A., BRUNTT H., GRUNDAHL F., FRANDSEN S., BEDIN L.R., MILONE A.P., DOTTER A., FEIDEN G.A., STETSON P.B., SANDQUIST E., MIGLIO A., STELLO D., JESSEN-HANSEN J.
	Astron. Astrophys., 543A, 106-106 (2012)
	Age and helium content of the open cluster NGC 6791 from multiple eclipsing binary members . II. Age dependencies and new insights.
o	photom.dat: <[BVB2012] NNNNN> N=15395 among (Nos 5810-33413).
=E=	Catalogue in electronic form as J/A+A/543/A106
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVC2003]
[BVC2003]	(Baume+Villanova+Carraro, 2003)
Write:	<<[BVC2003] Galaxy N>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Asiago observations. Discovery of 3 galaxies in the field of NGC 1663.
Ref:	=2003A&A...407..527B
by	BAUME G. , VILLANOVA S., CARRARO G.
	Astron. Astrophys., 407, 527-539 (2003)
	A study of the two northern open clusters NGC 1582 and NGC 1663.
o	Table 3, col(1): <Cl* NGC 1582 BVC NNN> (Nos 1-563). Table 5, col(1): <Cl* NGC 1663 BVC NNN> (Nos 1-131). Table 6: <[BVC2003] Galaxy N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVC2013]
[BVC2013]	(Benedettini+Viti+Codella+, 2013) (Not yet in Simbad)
Write:	<<[BVC2013] BNa-HVN>>
N:	4
Object:	High velocity bullet (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	IRAM PdB interferometer observations of N=4 high velocity bullets in the B1 shock in the LDN 1157 outflow.
in source:	LDN 1157: [DE95] LDN 1157 B1 = [DE95] LDN 1157 B1
Ref:	=2013MNRAS.436..179B
by	BENEDETTINI M. , VITI S., CODELLA C., GUETH F., GOMEZ-RUIZ A.I., BACHILLER R., BELTRAN M.T., BUSQUET G., CECCARELLI C., LEFLOCH B.
	Mon. Not. R. Astron. Soc., 436, 179-190 (2013)
	The B1 shock in the L1157 outflow as seen at high spatial resolution.
o	Fig. 4, Table 2: <[BVC2013] BNa-HVN> (Nos BOe-HV1, BOe-HV2, B1a-HV, B1b-HV).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVC99]
[BVC99]	(Botashev+Verkhodanov+Cardona+, 1999)
Write:	<<[BVC99] NNN>>
N:	115
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=115 galaxies in and near the cluster ACO 1185
in source:	ACO 1185
Ref:	=1999ARep...43...65B
by	BOTASHEV A.M. , VERKHODANOV O.V., CARDONA O., LIPOVKA N.M., LIPOVKA A.A., MINGALIEV M.G., CHAVIRA E.
	Astron. Rep., 43, 65-73 (1999)
	Investigation of galaxies in and near the cluster A1185.
o	Table 1: <[BVC99] NNN> (Nos 1-115).
=E=	Catalogue in electronic form as J/AZh/76/83
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVD2003]
[BVD2003]	(Boller+Voges+Dennefeld+, 2003) (Not yet in Simbad)
Write:	<<[BVD2003] N>>
N:	6
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	N=6 Chandra sources in the field of 1ES 1927+654.
Ref:	=2003A&A...397..557B
by	BOLLER T. , VOGES W., DENNEFELD M., LEHMANN I., PREDEHL P., BURWITZ V., PERLMAN E., GALLO L., PAPADAKIS I.E., ANDERSON S.
	Astron. Astrophys., 397, 557-564 (2003)
	1ES 1927+654: Persistent and rapid X-ray variability in an AGN with low intrinsic neutral X-ray absorption and narrow optical emission lines.
o	PDS 654 is misprint for PDS 456
o	Fig.9: <[BVD2003] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVD2011]
[BVD2011]	(Barentsen+Vink+Drew+, 2011)
Write:	<<[BVD2011] NNN>>
N:	158
Object:	Poss. T Tau * (SIMBAD class: TTauri*_Candidate = T Tauri Star Candidate)
Stat:	is completely incorporated in Simbad
Note:	Use of IPHAS observations of IC 1396 to identify N=158 T Tauri candidates in IC 1396.
in source:	IC 1396
Ref:	=2011MNRAS.415..103B
by	BARENTSEN G. , VINK J.S., DREW J.E., GREIMEL R., WRIGHT N.J., DRAKE J.J., MARTIN E.L., VALDIVIELSO L., CORRADI R.L.M.
	Mon. Not. R. Astron. Soc., 415, 103-132 (2011)
	T Tauri candidates and accretion rates using IPHAS: method and application to IC 1396.
o	Tables B1, C1: <[BVD2011] NNN> (Nos 1-158).
=E=	Catalogue in electronic form as <J/MNRAS/415/103/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BVF
BVF	(Bologna obs., Very Faint)= (BF)
Write:	<<BVF NNN>>
N:	298
Object:	UV Exc. Obj. (SIMBAD class: UV = UV-emission Source)
Note:	'The Bologna vf sample': in the 13h+36deg, 1.72 sq.deg selection u-b < - 0.1 or u-v < + 0.4 and b < 20.2 mag No Identif. chart, no cross-identif. The spectroscopic nature of several of these objects has been studied by Kron+, 1983A&A...127...29K
Ref:	=1980A&AS...39..129F
by	FORMIGGINI L. , ZITELLI V., BONOLI F., BRACCESI A.
	Astron. Astrophys., Suppl. Ser., 39, 129-132 (1980)
	A sample of very faint ultraviolet excess objets in the 13h + 36 field -I: the data.
o	No object in SIMBAD, the table is unreadable.
o	<BVF NNN> (Nos 1-298)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BVF2002]
[BVF2002]	(Best+Van Dokkum+Franx+, 2002)
Write:	<<[BVF2002] CNN>> <<[BVF2002] NNNN>>
Object:	G (SIMBAD class: Galaxy)
Note:	Radio observations of the Cluster ClG 1054-03 2002MNRAS.330...17B, table 3: comparison with HST observations, Old ID = [VFK98]. New ID = [BVF2002]. The new ID supersedes [VFK98]. Other 'NNNN' from the same list are found later in other references.
in source:	ClG 1054-0321 = 1E 1054.4-0321
Ref:	=2002MNRAS.330...17B
by	BEST P.N. , VAN DOKKUM P.G., FRANX M., ROETTGERING H.J.A.
	Mon. Not. R. Astron. Soc., 330, 17-34 (2002)
	µJy radio sources in the z=0.83 cluster MS1054-03.
o	Table 3: old ID = [VFK98] NNNN. p.19: calibrator 1058+015 = J1058+015 = RORF 1055+018. In ref list FANAROFF 1974MNRAS.167p..31F instead of 167.31
o	Table 1: <[BVF2002] CNN> (Nos C1-C34). Table 3, new ID: <[BVF2002] NNNN> N=27 among (Nos 1-6145).
Ref:	=2003ApJ...599..865T
by	TRAN K.-V.H. , FRANX M., ILLINGWORTH G., KELSON D.D., VAN DOKKUM P.
	Astrophys. J., 599, 865-885 (2003)
	The nature of E+A galaxies in intermediate-redshift clusters.
o	Table 4: designations of the galaxies in SIMBAD are: [FFF98] in ClG 1358+62, [TFI2003] in ClG 2053-04 (-03 is a misprint), [BVF2002] in ClG 1054-03.
o	Table 4: <[BVF2002] NNNN> N=19 added among (Nos 426-8001). Table 4: <[TFI2003] ClG 2053-04 NNNN> N=9 among (Nos 408-3549).
Ref:	=2004ApJ...605..677W
by	WUYTS S. , VAN DOKKUM P.G., KELSON D.D., FRANX M., ILLINGWORTH G.D.
	Astrophys. J., 605, 677-688 (2004)
	The detailed fundamental plane of two high-redshift clusters: MS 2053-04 at z=0.58 and MS 1054-03 at z=0.83.
o	Table 1: <[TFI2003] ClG 2053-04 NNNN> N=23 among (Nos 174-3549) added. Table 1: <[BVF2002] NNNN> N=18 added among (Nos 1192-6688).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVF96]
[BVF96]	(Barth+Van Dyk+Filippenko+, 1996)
Write:	<<[BVF96] A>> <<[BVF96] AN>>
N:	13
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST images Map in Fig. 1
in source:	M 83 = NGC 5236
Ref:	=1996AJ....111.2047B
by	BARTH A.J. , VAN DYK S.D., FILIPPENKO A.V., LEIBUNDGUT B., RICHMOND M.W.
	Astron. J., 111, 2047-2058 (1996)
	The environments of supernovae in archival Hubble Space Telescope images.
o	Table 2: <[BVF96] AN> (Nos A1-A7, B, C1-C4, N)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVG83]
[BVG83]	(Baryshev+Vitkovskij+Gol'nev+, 1983)
Write:	<<[BVG83] NN>>
N:	57
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Observations with the Ratan-600 radio telescope
Ref:	=1983AZh....60.1084B
by	BARYSHEV Y.V. , VITKOVSKIJ V.V., GOL'NEV V.Y., KONONOV V.K., LIPOVKA N.M., PETROV Z.E.
	Astron. Zh., 60, 1084-1090 (1983)
	The results of observations of the giant HII region at the longitude of l = 4-10 carried out with high resolution.
o	Table I: <[BVG83] NN> (Nos 1-57)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVH2007]
[BVH2007]	(Burenin+Vikhlinnin+Hornstrup+, 2007)
Write:	<<[BVH2007] NNN>> <<[BVH2007] 5-NN>> <<[BVH2007] JHHMMSS.s+DDMMSS>>
N:	242+24+5
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC catalog of high redshift clusters at target redshift. Table 6: Other extended sources.
Ref:	=2007ApJS..172..561B
by	BURENIN R.A. , VIKHLININ A., HORNSTRUP A., EBELING H., QUINTANA H., MESCHERYAKOV A.
	Astrophys. J., Suppl. Ser., 172, 561-582 (2007)
	The 400 square ° ROSAT PSPC galaxy cluster survey: catalog and statistical calibration.
o	Table 4: <[BVH2007] NNN> (Nos 1-242). Table 5: <[BVH2007] 5-NN> (Nos 5-1 to 5-24). Table 6: <[BVH2007] JHHMMSS.s+DDMMSS> N=5.
=E=	Catalogue in electronic form as J/ApJS/172/561
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVK2003]
[BVK2003]	(Bassa+Van Kerkwijk+Kulkarni, 2003)
Write:	<<[BVK2003] A>>
N:	10
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Keck observations. N=10 stars in the field of PSR J0218+4232. Star X is the pulsar companion, star Y is 2" west of the PSR.
Ref:	=2003A&A...403.1067B
by	BASSA C.G. , VAN KERKWIJK M.H., KULKARNI S.R.
	Astron. Astrophys., 403, 1067-1075 (2003)
	Temperature and cooling age of the white dwarf companion of PSR J0218+4232.
o	Table 3: <[BVK2003] A> (Nos A-H, X, Y).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVK2006]
[BVK2006]	(Bassa+Van Kerkwijk+Kulkarni, 2006)
Write:	<<[BVK2006] A>>
N:	8+1
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Optical and near-IR observations with Keck of PSR J0751+1807 with LRIS and ESI on Keck I and II. N=9 stars are observed in the field of the pulsar, (Nos A-H, X). The star X is the white dwarf companion of the pulsar.
Ref:	=2006A&A...450..295B
by	BASSA C.G. , VAN KERKWIJK M.H., KULKARNI S.R.
	Astron. Astrophys., 450, 295-303 (2006)
	The ultra-cool white dwarf companion of PSR J0751+1807.
o	Fig.1, Table 2: <[BVK2006] A> (Nos A-H, X).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVK2006a]
[BVK2006a]	(Bassa+Van Kerkwijk+Kulkarni, 2006)
*****	Avoid the usage of [BVK2006a], prefer [BVK2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVK2006b]
[BVK2006b]	(Bassa+Van Kerkwijk+Koester+, 2006)
Write:	<<[BVK2006b] A>>
N:	5
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS1 observations of reference stars near PSR J1911-5958A.
Ref:	=2006A&A...456..295B
by	BASSA C.G. , VAN KERKWIJK M.H., KOESTER D., VERBUNT F.
	Astron. Astrophys., 456, 295-304 (2006)
	The masses of PSR J1911-5958A and its white dwarf companion.
o	Star WD is NAME COM J1911-5958A in Simbad.
o	Fig.2, Table 1: <[BVK2006b] A> (Nos A-D, R).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVM2014]
[BVM2014]	(Banados+Venemans+Morganson+, 2014)
Write:	<<[BVM2014] J224059.407-183934.94>>
N:	1
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	APEX LABOCA 870µm observations of N=1 submillimeter source at ∼2.5' from PSO J340.2041-18.6621.
Ref:	=2014AJ....148...14B
by	BANADOS E. , VENEMANS B.P., MORGANSON E., DECARLI R., WALTER F., CHAMBERS K.C., RIX H.-W., FARINA E.P., FAN X., JIANG L., McGREER I., DE ROSA G., SIMCOE R., WEISS A., PRICE P.A., MORGAN J.S., BURGETT W.S., GREINER J., KAISER N., KUDRITZKI R.-P., MAGNIER E.A., METCALFE N., STUBBS C.W., SWEENEY W., TONRY J.L., WAINSCOAT R.J., WATERS C.
	Astron. J., 148, 14 (2014)
	Discovery of eight z ~ 6 quasars from Pan-STARRS1.
o	Appendix B: <[BVM2014] J224059.407-183934.94> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVM98]
[BVM98]	(Belloni+Verbunt+Mathieu, 1998)
Write:	<<[BVM98] M 67 NN>> <<[BVM98] NGC 188 NN>>
N:	59+34
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Table 1: Sources in M 67. Sources (Nos 1-22): see BVS. Sources BVS 5 and 20 are not found here, and have been discarded. Table 2: Sources in NGC 188.
in source:	M 67 = NGC 2682
in source:	NGC 188
Ref:	=1998A&A...339..431B
by	BELLONI T. , VERBUNT F., MATHIEU R.D.
	Astron. Astrophys., 339, 431-439 (1998)
	X-rays from old open clusters: M 67 and NGC 188.
o	(Erratum) Erratum vol. 351, p. 398 (1999)
o	Table 1: <[BVM98] M 67 NN> N=59, (Nos 1-4, 6-19, 21-61). Table 2: <[BVM98] NGC 188 NN (Nos 1-34).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BVMC
BVMC	(Bordeaux and Vahinhos Meridian Circle catalogue)
Write:	<<BVMC JHHMMSS.sss+DDMMSS.ss>>
N:	546459
Object:	* (SIMBAD class: Star)
Note:	Extension of VMCC catalog with small differences in coordinates.
Ref:	=2003A&A...409..361C
by	CAMARGO J.I.B. , DUCOURANT C., TEIXEIRA R., LE CAMPION J.-F., RAPAPORT M., BENEVIDES-SOARES P.
	Astron. Astrophys., 409, 361-368 (2003)
	Extension of the ICRF for selected areas down to the 16th magnitude - II.
o	Catalog: <BVMC JHHMMSS.sss+DDMMSS.ss> N=546459.
=E=	Catalogue in electronic form as J/A+A/409/361
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BVP2001]
[BVP2001]	(Burenin+Vikhlinin+Pavlinsky, 2001) (Not yet in Simbad)
Write:	<<[BVP2001] JHHMM+DDMM>>
N:	8
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	ROSAT X-ray survey of clusters. See also [VMF98].
Ref:	=2001AstL...27..557B
by	BURENIN R.A. , VIKHLININ A.A., PAVLINSKY M.N.
	Astron. Lett., 27, 557-561 (2001)
	Photometric observations of galaxy clusters from a new X-ray survey.
o	Table 2: format J2000 or B1950?
o	Table 2: <[BVP2001] JHHMM+DDMM> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVP2003]
[BVP2003]	(Blomme+Van de Steene+Prinja+, 2003)
Write:	<<[BVP2003] SN>>
N:	6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ATCA image of the field around the star zet Pup.
Ref:	=2003A&A...408..715B
by	BLOMME R. , VAN DE STEENE G.C., PRINJA R.K., RUNACRES M.C., CLARK J.S.
	Astron. Astrophys., 408, 715-727 (2003)
	Radio and submillimetre observations of wind structure in ζ Puppis.
o	Table 4: <[BVP2003] SN> (Nos S2-S7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVP2004]
[BVP2004]	(Barnard+Vielva+Pierce-Price+, 2004)
Write:	<<[BVP2004] gc N>> <<[BVP2004] per NN>>
N:	6+15
Object:	(submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SCUBA results of a search for bright high-redshift galaxies in the Galactic Center and the Perseus Region. N=6 and 15 point sources candidates are observed. No extragalactic source found.
in source:	NAME Gal Center
in source:	NAME Per Region
Ref:	=2004MNRAS.352..961B
by	BARNARD V.E. , VIELVA P., PIERCE-PRICE D.P.I., BLAIN A.W., BARREIRO R.B., RICHER J.S., QUALTROUGH C.
	Mon. Not. R. Astron. Soc., 352, 961-974 (2004)
	The very bright SCUBA galaxy count: looking for SCUBA galaxies with the Mexican hat wavelet.
o	Table 2: <[BVP2004] gc N> (Nos 1-6), <[BVP2004] per NN> (Nos 1-15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVR2013]
[BVR2013]	(Balestra+Vanzella+Rosati+, 2014)
Write:	<<[BVR2013] JHHMMSS.ss+DDMMSS.s>>
N:	15
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	VLT VIMOS observations of N=15 strong-lensing features and magnified background sources targeted in the galaxy cluster RXC J2248.0-4431.
in source:	RXC J2248.0-4431
Ref:	=2013A&A...559L...9B
by	BALESTRA I. , VANZELLA E., ROSATI P., MONNA A., GRILLO C., NONINO M., MERCURIO A., BIVIANO A., BRADLEY L., COE D., FRITZ A., POSTMAN M., SEITZ S., SCODEGGIO M., TOZZI P., ZHENG W., ZIEGLER B., ZITRIN A., ANNUNZIATELLA M., BARTELMANN M., BENITEZ N., BROADHURST T., BOUWENS R., CZOSKE O., DONAHUE M., FORD H., GIRARDI M., INFANTE L., JOUVEL S., KELSON D., KOEKEMOER A., KUCHNER U., LEMZE D., LOMBARDI M., MAIER C., MEDEZINSKI E., MELCHIOR P., MENEGHETTI M., MERTEN J., MOLINO A., MOUSTAKAS L., PRESOTTO V., SMIT R., UMETSU K.
	Astron. Astrophys., 559L, 9-9 (2013)
	CLASH-VLT: spectroscopic confirmation of a z = 6.11 quintuply lensed galaxy in the Frontier Fields cluster RXC J2248.7-4431.
o	(Erratum) erratum vol. 611, art. C2 (2018)
o	Table 1: <[BVR2013] JHHMMSS.ss+DDMMSS.s> N=15.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BVS
BVS	(Belloni+Verbunt+Schmitt)= (B) = ([BVS93])
Write:	<<BVS NNa>>
N:	22+2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations See [PB98] for possible optical identifications. See [BVM98].
in source:	M 67 = NGC 2682
Ref:	=1993A&A...269..175B
by	BELLONI T. , VERBUNT F., SCHMITT J.H.M.M.
	Astron. Astrophys., 269, 175-180 (1993)
	ROSAT detection of stellar X-ray sources in the old open cluster M 67.
o	Table 1: <BVS NN> (Nos 1-22)
Ref:	=1998A&A...336..902P
by	PASQUINI L. , BELLONI T.
	Astron. Astrophys., 336, 902-910 (1998)
	Optical identification of ROSAT sources in M 67: activity in an old cluster.
o	<BVS NNa> (Nos 11a-11b). <[PB98] BNN-A> (Nos B1-A, B1-B, B2-A, B2-B, B15-A).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BVS93]
[BVS93]	(Belloni+Verbunt+Schmitt, 1993)
*****	Avoid the usage of [BVS93], prefer BVS
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVV2021]
[BVV2021]	(Busekool+Verheijen+van der Hulst+, 2021)
Write:	<<[BVV2021] UMa-HINN>>
N:	17
Object:	HI G (SIMBAD class: Galaxy)
Note:	VLA observations of N=17 HI-detected galaxies in the Ursa Major (UMa) volume.
in source:	NAME UMa Cluster
Ref:	=2021MNRAS.501.2608B
by	BUSEKOOL E. , VERHEIJEN M.A.W., VAN DER HULST J.M., TULLY R.B., TRENTHAM N., ZWAAN M.A.
	Mon. Not. R. Astron. Soc., 501, 2608-2626 (2021)
	The Ursa Major association of galaxies - VI: a relative dearth of gas-rich dwarf galaxies.
o	Figs A1-A2, Table 4: <[BVV2021] UMa-HINN> (Nos HI01-HI17).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVW2006]
[BVW2006]	(Bremer+Valtchanov+Willis+, 2006)
Write:	<<[BVW2006] GN>>
N:	7
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	CFHTLS, NTT SOFI, and VLT FORS observations of XLSSU J022303.0-043622.
in source:	XLSSU J022303.0-043622
Ref:	=2006MNRAS.371.1427B
by	BREMER M.N. , VALTCHANOV I., WILLIS J., ALTIERI B., ANDREON S., DUC P.A., FANG F., JEAN C., LONSDALE C., PACAUD F., PIERRE M., SHUPE D.L., SURACE J.A., WADDINGTON I.
	Mon. Not. R. Astron. Soc., 371, 1427-1434 (2006)
	XMM-LSS discovery of a z = 1.22 galaxy cluster.
o	Fig.1, Table 1: <[BVW2006] GN> (Nos G1-G7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BVW2013]
[BVW2013]	(Banados+Venemans+Walter+, 2013)
Write:	<<[BVW2013] LAE N>> <<[BVW2013] Drop N>>
N:	10
Object:	LAE + LBG (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 observations of N=10 Lymanα emitters (LAEs) and Lyman break galaxies (LBGs) around the quasar ULAS J0203+0012 at z∼5.7. Use of archival SDF data. See also [MBD2017].
in source:	QSO J0203+0012
Ref:	=2013ApJ...773..178B
by	BANADOS E. , VENEMANS B., WALTER F., KURK J., OVERZIER R., OUCHI M.
	Astrophys. J., 773, 178 (2013)
	The galaxy environment of a QSO at z ~ 5.7.
o	Table 1: <[BVW2013] LAE N> N=2, <BVW2013] Drop N> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BW
BW	(Not yet in Simbad)
*****	Avoid the usage of BW, prefer [JWM2012]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BW
BW	(Baade's Window)
*****	Avoid the usage of BW, prefer [B84]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BW
BW	(Bar West)
*****	Avoid the usage of BW, prefer BMB-BW
Details on Acronym: BW
BW	(Berkhuijsen+Wielebinski)
*****	Avoid the usage of BW, prefer [BW74]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BW
BW	(Bohuski+Weedman)
*****	Avoid the usage of BW, prefer BW79
Origin	of the Acronym: L = Found in the literature
Details on Acronym: BW
BW	(Becker+White)
*****	Avoid the usage of BW, prefer [BW88]
Origin	of the Acronym: L (1998AJ....116..890S)
Details on Acronym: BW
BW	(Baade Window)
*****	Avoid the usage of BW, prefer [GGA99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BW
BW	(Baade's window)
*****	Avoid the usage of BW, prefer [RG96]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BW
BW	(Baade's window)
*****	Avoid the usage of BW, prefer [RT92]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BW2
BW2	(Baade's window, list 2)
*****	Avoid the usage of BW2, prefer [RT93]
Origin	of the Acronym: L (1992A&AS...95..379R)
Details on Acronym: [BW2000]
[BW2000]	(Berghofer+Wendker, 2000)
Write:	<<[BW2000] NN>>
N:	11
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations of the field around P Cyg.
Ref:	=2000AN....321..249B
by	BERGHOEFER T.W. , WENDKER H.J.
	Astron. Nachr., 321, 249-253 (2000)
	ROSAT HRI observations of P Cyg and surrounding area.
o	Table 1: <[BW2000] NN> (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BW2007]
[BW2007]	(Brand+Wouterloot, 2007)
Write:	<<[BW2007] NN>>
N:	63
Object:	* (SIMBAD class: Star)
Note:	ESO 2.2m telescope NIR observations of IRAS 06145+1455.
in source:	W89 789 = IRAS 06145+1455
Ref:	=2007A&A...464..909B
by	BRAND J. , WOUTERLOOT J.G.A.
	Astron. Astrophys., 464, 909-920 (2007)
	A star cluster at the edge of the Galaxy.
o	Table 4: <[BW2007] NN> N=63 among (Nos 1-99).
=E=	Catalogue in electronic form as J/A+A/464/909
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BW2010]
[BW2010]	(Beaumont+Williams, 2010)
Write:	<<[BW2010] NN>>
N:	12
Object:	Outflow (SIMBAD class: Outflow)
Stat:	is completely incorporated in Simbad
Note:	JCMT CO(3-2) observations of N=12 outflows in ISM cavities in the Galactic plane.
Ref:	=2010ApJ...709..791B
by	BEAUMONT C.N. , WILLIAMS J.P.
	Astrophys. J., 709, 791-800 (2010)
	Molecular rings around interstellar bubbles and the thickness of star-forming clouds.
o	Table 4: <[BW2010] NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BW2019]
[BW2019]	(Brunetti+Wilson, 2019)
Write:	<<[BW2019] 30 Dor-10 NN>> <<[BW2019] N159W N>> <<[BW2019] N159E N>>
N:	32
Object:	Clump (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	ALMA bands 3 and 6 continuum observations of N=32 molecular clumps in N=3 star-forming regions in the LMC.
in source:	[JGB98] 30 Dor-10
in source:	LHA 120-N 159W
in source:	LHA 120-N 159E
Ref:	=2019MNRAS.483.1624B
by	BRUNETTI N. , WILSON C.D.
	Mon. Not. R. Astron. Soc., 483, 1624-1641 (2019)
	An ALMA archival study of the clump mass function in the Large Magellanic Cloud.
o	Table 4: <[BW2019] 30 Dor-10 NN> (Nos 1-22), <[BW2019] N159W N> (Nos 1-7), <[BW2019] N159E N> (Nos 1-3).
o	PCC 11546 is PGCC G282.98-32.40 in Simbad.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BW59]
[BW59]	(Blanco+Williams, 1959) (Not yet in Simbad)
Write:	<<[BW59] NN>>
N:	16
Object:	* (SIMBAD class: Star)
Note:	Superseded by 'MacC NN'
in source:	NAME Cepheus IV
Ref:	=1959ApJ...130..482B
by	BLANCO V.M. , WILLIAMS A.D.
	Astrophys. J., 130, 482-486 (1959)
	A new OB association with an unusual reddening effect.
o	misprint in table 1 star 5 read BD +67 1580
o	[BW59] superseded by <MacC NN> here (Nos 1-16)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BW74]
[BW74]	(Berkhuijsen+Wielebinski, 1974)= (BW)
Write:	<<[BW74] N>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
in source:	M 31 = NGC 224
Ref:	=1974A&A....34..173B
by	BERKHUIJSEN E.M. , WIELEBINSKI R.
	Astron. Astrophys., 34, 173-179 (1974)
	A radio continuum survey of M 31 at 2695 MHz.
o	Table 2: <[BW74] N> (Nos 1-4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BW79
BW79	(Bohuski+Weedman, 1979)= (BW)
Write:	<<BW79 NN>>
N:	23
Object:	EmG + QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Note:	Table 2: (Nos 1-23), cross-id. with Tol HHMM.m+DD.d.
Ref:	=1979ApJ...231..653B
by	BOHUSKI T.J. , WEEDMAN D.W.
	Astrophys. J., 231, 653-658 (1979)
	Limits on the number of faint quasars.
o	Table 2, col (1): <BW79 NN> (Nos 1-23) = Table 2, col (2): <Tol HHMM.m-DD.d> N=23.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BW88]
[BW88]	(Becker+White, 1988)= (BW) = (Lick) = (VLA)
Write:	<<[BW88] N>>
N:	9
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio objects near LkHA 101
Ref:	=1988ApJ...324..893B
by	BECKER R.H. , WHITE R.L.
	Astrophys. J., 324, 893-898 (1988)
	LkH-α 101: the stellar wind, the surrounding nebula and an associated star cluster.
o	Table 2: <[BW88] N> (Nos 1-9)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BW89]
[BW89]	(Bell+Whitmore, 1989)= (WR)
Write:	<<[BW89] NNN>>
N:	174
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	DRCG 1842-63
Ref:	=1989ApJS...70..139B
by	BELL M. , WHITMORE B.C.
	Astrophys. J., Suppl. Ser., 70, 139-161 (1989)
	Photometric properties of galaxies in the cluster DC 1842-63.
o	<[BW89] NNN> N=174
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BW93]
[BW93]	(Birkinshaw+Worrall, 1993)
Write:	<<[BW93] NGC 6251 A>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT observations of the radio jet of NGC 6251. NGC 6251 A-D are features in the radio jet.
Ref:	=1993ApJ...412..568B
by	BIRKINSHAW M. , WORRALL D.M.
	Astrophys. J., 412, 568-585 (1993)
	The X-ray structure and spectrum of NGC 6251.
o	Table 1: <[BW93] NGC 6251 A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BW95]
[BW95]	(Bower+Wilson, 1995)
Write:	<<[BW95] A>> <<[BW95] Nuclear>>
N:	5+1
Object:	Cluster of * + (Rad) (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST Planetary Camera Table 3: N=5 Cl* (Nos A-E) Table 5: N=1 radio-source '[BW95] Nuclear'
in source:	NGC 5930
Ref:	=1995ApJS...99..543B
by	BOWER G.A. , WILSON A.S.
	Astrophys. J., Suppl. Ser., 99, 543-549 (1995)
	Hubble Space Telescope images of the nuclear star-forming region in the interacting galaxy NGC 5930.
o	Table 3: <[BW95] A> (Nos A-E), Table 5: <[BW95] Nuclear> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BW98]
[BW98]	(Brand+Wouterloot, 1998) (Not yet in Simbad)
Write:	<<[BW98] Cloud A>> <<[BW98] Ridge N>> <<[BW98] Clump W>>
N:	5+2+2
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Study of the area around Sh 2-151.
in source:	SH 2-151
Ref:	=1998A&A...337..539B
by	BRAND J. , WOUTERLOOT J.G.A.
	Astron. Astrophys., 337, 539-557 (1998)
	A multi-wavelength study of the Sharpless 151 region.
o	H2O maser = EQ 2300+5641
o	Table 3: <[BW98] Cloud A> (Nos A-D). Table 5: <[BW98] Ridge N> (Nos 1-2), [BW98] > (Nos N, S).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWA2004]
[BWA2004]	(Becker+Weisskopf+Arzoumanian+, 2004)
Write:	<<[BWA2004] AFNN>>
N:	38
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra sources in the field of gam Cyg.
Ref:	=2004ApJ...615..897B
by	BECKER W. , WEISSKOPF M.C., ARZOUMANIAN Z., LORIMER D., CAMILO F., ELSNER R.F., KANBACH G., REIMER O., SWARTZ D.A., TENNANT A.F., O'DELL S.L.
	Astrophys. J., 615, 897-907 (2004)
	A multiwavelength search for a counterpart of the brightest unidentified γ-ray source 3EG J2020+4017 (2CG 078+2).
o	Table 1: <[BWA2004] SFNN> N=19+16+3.
=E=	Catalogue in electronic form as J/ApJ/615/897
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWB2019]
[BWB2019]	(Bait+Wadadekar+Barway, 2019)
Write:	<<[BWB2019] XN.N>>
N:	6
Object:	Em. Obj. (SIMBAD class: EmObj = Emission Object)
Stat:	is completely incorporated in Simbad
Note:	N=6 extended Hα emitters associated with five MaNGA galaxies. Use of SDSS DR14, DECaLS DR5, and MzLS/BASS DR6 data.
Ref:	=2019MNRAS.485..428B
by	BAIT O. , WADADEKAR Y., BARWAY S.
	Mon. Not. R. Astron. Soc., 485, 428-439 (2019)
	Outlying Hα emitters in SDSS IV MaNGA.
o	Tables 1-2: <[BWB2019] XN.N> (Nos X1, X2.1-X2.2, X3-X5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWB83]
[BWB83]	(Batrla+Wilson+Bastien+, 1983)
Write:	<<[BWB83] SN>>
N:	6
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Note:	Fig.1 and Table 1: sources are found in the literature as 'Ori SN' or 'Ori S-N'
in source:	NAME Orion Nebula
Ref:	=1983A&A...128..279B
by	BATRLA W. , WILSON T.L., BASTIEN P., RUF K.
	Astron. Astrophys., 128, 279-290 (1983)
	Clumping in molecular clouds. The region between OMC 1 and 2.
o	<[BWB83] SN> (Nos S1-S6)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWC2006]
[BWC2006]	(Bains+Wong+Cunningham+, 2006)
Write:	<<[BWC2006] 13CO NN>> <<[BWC2006] mm NNN>>
N:	61+105
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Note:	ATNF Mopra telescope 13CO observations of the region of RCW 106. Properties of the mm dust clumps associated with 13CO measures.
in source:	RCW 106
Ref:	=2006MNRAS.367.1609B
by	BAINS I. , WONG T., CUNNINGHAM M., SPARKS P., BRISBIN D., CALISSE P., DEMPSEY J.T., DERAGOPIAN G., ELLINGSEN S., FULTON B., HERPIN F., JONES P., KOUBA Y., KRAMER C., LADD E.F., LONGMORE S.N., McEVOY J., MALLER M., MINIER V., MOOKERJEA B., PHILLIPS C., PURCELL C.R., WALSH A., VORONKOV M.A., BURTON M.G.
	Mon. Not. R. Astron. Soc., 367, 1609-1628 (2006)
	Molecular line mapping of the giant molecular cloud associated with RCW 106 - I. ^{13}CO.
o	Table 1: <[BWC2006] 13CO NN> (Nos 1-61). Table 3: <[BWC2006] mm NNN> N=105 among (Nos 1-138).
=E=	Catalogue in electronic form as J/MNRAS/367/1609
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWC2008]
[BWC2008]	(Berghea+Weaver+Colbert+, 2008)
Write:	<<[BWC2008] UNN>> <<[BWC2008] CNN>>
N:	26
Object:	(X) (SIMBAD class: ULX = Ultra-luminous X-ray Source)
Note:	Archival Chandra data of ULX sources.
Ref:	=2008ApJ...687..471B
by	BERGHEA C.T. , WEAVER K.A., COLBERT E.J.M., ROBERTS T.P.
	Astrophys. J., 687, 471-487 (2008)
	Testing the paradigm that ultraluminous X-ray sources as a class represent accreting intermediate-mass black holes.
o	Table 2, col(2): <[BWC2008] UNN> (Nos U1-U47), <[BWC2008] CNN> (Nos C1-C22).
=E=	Catalogue in electronic form as <J/ApJ/687/471/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWC2021]
[BWC2021]	(Barnett+Warren+Cross+, 2021)
Write:	<<[BWC2021] JHHMMSS.ss+DDMMSS.s>>
N:	32
Object:	Poss. High redshift QSO (SIMBAD class: AGN_Candidate = Active Galaxy Nucleus Candidate)
Note:	N=32 high-redshift quasar candidates (6.5<z<9.3) in 977 sq. deg. of the VIKING survey. Use of DESI Legacy Survey, VST ATLAS survey, KiDS survey, and Pan-STARRS data.
Ref:	=2021MNRAS.501.1663B
by	BARNETT R. , WARREN S.J., CROSS N.J.G., MORTLOCK D.J., FAN X., WANG F., HEWETT P.C.
	Mon. Not. R. Astron. Soc., 501, 1663-1676 (2021)
	A complete search for redshift z >= 6.5 quasars in the VIKING survey.
o	Table 1: <[BWC2021] JHHMMSS.ss+DDMMSS.s> N=32.
o	Table 1 : VIKING sources from DR 2016-04-06 according to Section 2; however only 9 out of the 17 "Candidates" do exist in the VIKING release 2 (2016-10-10, II/343/viking2 in VizieR).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWD2008]
[BWD2008]	(Brand+Weedman+Desai+, 2008)= (70Bootes) = ([BWD2008a]) = (SST24)
Write:	<<[BWD2008] 70BootesNN>> <<[BWD2008] SST24 JHHMMSS.s+DDMMSS>>
N:	11+15
Object:	IR G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spitzer MIPS survey of the NDWFS Bootes field at 70mu.m.
in source:	NAME Bootes Field
Ref:	=2008ApJ...673..119B
by	BRAND K. , WEEDMAN D.W., DESAI V., LE FLOC'H E., ARMUS L., DEY A., HOUCK J.R., JANNUZI B.T., SMITH H.A., SOIFER B.T.
	Astrophys. J., 673, 119-127 (2008)
	Spitzer mid-infrared spectroscopy of 70 µm-selected distant luminous infrared galaxies.
o	Table 1: <[BWD2008] 70BootesNN> (Nos 1-11) = <[BWD2008] SST24 JHHMMSS.s+DDMMSS> N=11.
Ref:	=2008ApJ...680..119B
by	BRAND K. , WEEDMAN D.W., DESAI V., LE FLOC'H E., ARMUS L., DEY A., HOUCK J.R., JANNUZI B.T., SMITH H.A., SOIFER B.T.
	Astrophys. J., 680, 119-129 (2008)
	Spitzer mid-infrared spectroscopy of distant X-ray luminous active galactic nuclei.
o	Table 1, col(1): <[BWD2008b] Bootes XNN> (Nos X1-X15) = Table 1, col(2): <[BWD2008] SST24 JHHMMSS.s+DDMMSS> N=15.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWD2008a]
[BWD2008a]	(Brand+Weedman+Desai+, 2008)
*****	Avoid the usage of [BWD2008a], prefer [BWD2008]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWD2008b]
[BWD2008b]	(Brand+Weedman+Desai+, 2008)= (Bootes) = (SST24)
Write:	<<[BWD2008b] Bootes XNN>>
N:	15
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRS observations of N=16 optically faint infrared luminous galaxies in the NAO Deep Wide-Field Survey Bootes field.
in source:	NAME Bootes Field
Ref:	=2008ApJ...680..119B
by	BRAND K. , WEEDMAN D.W., DESAI V., LE FLOC'H E., ARMUS L., DEY A., HOUCK J.R., JANNUZI B.T., SMITH H.A., SOIFER B.T.
	Astrophys. J., 680, 119-129 (2008)
	Spitzer mid-infrared spectroscopy of distant X-ray luminous active galactic nuclei.
o	Table 1, col(1): <[BWD2008b] Bootes XNN> (Nos X1-X15) = Table 1, col(2): <[BWD2008] SST24 JHHMMSS.s+DDMMSS> N=15.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BWE
BWE	(Becker+White+Edwards)
Write:	<<BWE HHMM+DDMMA>>
N:	53522
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Catalog of 53522 sources at 4.85 GHz between 0deg and 75deg declination, generated from observations taken with the NRAO Green Bank 300 foot (91m) telescope by Condon et al. (1989 AJ 97 1064). The same data were used for 87GB, ref. 1991ApJS...75.1011G
Ref:	=1991ApJS...75....1B
by	BECKER R.H. , WHITE R.L., EDWARDS A.L.
	Astrophys. J., Suppl. Ser., 75, 1-229 (1991)
	A new catalog of 53,522 4.85 GHz sources.
o	Table 3: <BWE HHMM+DDMMA> N=53522
=E=	Catalogue in electronic form as VIII/13
=E=	Catalogue in electronic form as VIII/14
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BWE2009]
[BWE2009]	(Belokurov+Walker+Evans+, 2009)
Write:	<<[BWE2009] Seg2-NNN>>
N:	352
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	MMT Megacam imaging and Hectochelle spectroscopy of a new Milky Way satellite.
in source:	NAME Segue 2
Ref:	=2009MNRAS.397.1748B
by	BELOKUROV V. , WALKER M.G., EVANS N.W., GILMORE G., IRWIN M.J., MATEO M., MAYER L., OLSZEWSKI E., BECHTOLD J., PICKERING T.
	Mon. Not. R. Astron. Soc., 397, 1748-1755 (2009)
	The discovery of Segue 2: a prototype of the population of satellites of satellites.
o	Text, Table 1: <NAME Segue 2>. Table 2: <[BWE2009] Seg2-NNN> (Nos 1-352).
=E=	Catalogue in electronic form as J/MNRAS/397/1748
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWE2010]
[BWE2010]	(Bunker+Wilkins+Ellis+, 2010)
Write:	<<[BWE2010] zDNN>> <<[BWE2010] YDN>>
N:	12+7
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFC3 observations of galaxies at z∼7-10 in the Hubble Ultra Deep Field.
in source:	NAME HUDF
Ref:	=2010MNRAS.409..855B
by	BUNKER A.J. , WILKINS S., ELLIS R.S., STARK D.P., LORENZONI S., CHIU K., LACY M., JARVIS M.J., HICKEY S.
	Mon. Not. R. Astron. Soc., 409, 855-866 (2010)
	The contribution of high-redshift galaxies to cosmic reionization: new results from deep WFC3 imaging of the Hubble Ultra Deep Field.
o	Fig. 1, Table 1: <[BWE2010] zDNN> (Nos 0-11). Fig. 7, Table 2: <[BWE2010] YDN> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWE2012]
[BWE2012]	(Binder+Williams+Eracleous+, 2012)
Write:	<<[BWE2012] NGC 300 NN>>
N:	95
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS observations of N=95 X-ray point sources of NGC 300, as part of the Chandra Local Volume Survey. See also CXOLV, [BWE2013] and [BWE2015].
in source:	NGC 300
Ref:	=2012ApJ...758...15B
by	BINDER B. , WILLIAMS B.F., ERACLEOUS M., GAETZ T.J., PLUCINSKY P.P., SKILLMAN E.D., DALCANTON J.J., ANDERSON S.F., WEISZ D.R., KONG A.K.H.
	Astrophys. J., 758, 15 (2012)
	The Chandra Local Volume Survey: the X-ray point-source catalog of NGC 300.
o	Tables 4-7, Col(ID): <CXOLV JHHMMSS.ss+DDMMSS.s> N=95 = Tables 4-7, Col(Seq): <[BWE2012] NGC 300 NN> (Nos 1-95).
=E=	Catalogue in electronic form as J/ApJ/758/15
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWE2013]
[BWE2013]	(Binder+Williams+Eracleous+, 2013)
Write:	<<[BWE2013] NGC 404 NN>>
N:	74
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS-S observations of N=74 X-ray point sources of NGC 404, as part of the Chandra Local Volume Survey. See also CXOLV, [BWE2012] and [BWE2015].
in source:	NGC 404
Ref:	=2013ApJ...763..128B
by	BINDER B. , WILLIAMS B.F., ERACLEOUS M., GAETZ T.J., KONG A.K.H., SKILLMAN E.D., WEISZ D.R.
	Astrophys. J., 763, 128 (2013)
	The Chandra local volume survey: the X-ray point-source population of NGC 404.
o	Tables 3-6, 10, 13, Col(ID): <CXOLV JHHMMSS.ss+DDMMSS.s> N=74 = Tables 3-6, 10, 13, Col(Seq): <[BWE2013] NGC 404 NN> (Nos 1-74).
=E=	Catalogue in electronic form as J/ApJ/763/128
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWE2015]
[BWE2015]	(Binder+Williams+Eracleous+, 2015)
Write:	<<[BWE2015] NGC NNNN NNN>>
N:	460
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS observations of N=154+190+113 X-ray point sources of NGC 55, NGC 2403 and NGC 4214 as part of the Chandra Local Volume Survey. See also CXOLV, [BWE2012] and [BWE2013].
in source:	NGC 55
in source:	NGC 2403
in source:	NGC 4214
Ref:	=2015AJ....150...94B
by	BINDER B. , WILLIAMS B.F., ERACLEOUS M., PLUCINSKY P.P., GAETZ T.J., ANDERSON S.F., SKILLMAN E.D., DALCANTON J.J., KONG A.K.H., WEISZ D.R.
	Astron. J., 150, 94 (2015)
	The Chandra Local Volume Survey. I. The X-ray point source populations of NGC 55, NGC 2403, and NGC 4214.
o	Table 5: <CXOLV JHHMMSS.ss+DDMMSS.s> N=967. Tables 8, 20 : <[BWE2015] NGC NNNN NNN> N=460.
=E=	Catalogue in electronic form as J/AJ/150/94
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWE97]
[BWE97]	(Boyle+Wilkes+Elvis, 1997)
Write:	<<[BWE97] JHHMMSS.s+DDMMSS>>
N:	120
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	WHT ISIS spectroscopy of ROSAT PSPC sources in the CRSS survey.
Ref:	=1997MNRAS.285..511B
by	BOYLE B.J. , WILKES B.J., ELVIS M.
	Mon. Not. R. Astron. Soc., 285, 511-528 (1997)
	The Cambridge-Cambridge ROSAT Serendipity Survey - V. Catalogue and optical identifications.
o	Table 2: <CRSS JHHMM.m+DDMM> N=123, <[BWE97] JHHMMSS.s+DDMMSS> N=120.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWF97]
[BWF97]	(Brandt+Ward+Fabian+, 1997)
Write:	<<[BWF97] IC 10 X-N>> <<[BWF97] N>>
N:	1+3+2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations Text: N=1 X-ray source in IC 10, format 'IC 10 X-1' Table 1: N=5 X-ray sources, (Nos 1-5), (Nos 1-3) are near NGC 147, (Nos 4-5) are near NGC 185.
in source:	IC 10
in source:	NGC 147
in source:	NGC 185
Ref:	=1997MNRAS.291..709B
by	BRANDT W.N. , WARD M.J., FABIAN A.C., HODGE P.W.
	Mon. Not. R. Astron. Soc., 291, 709-716 (1997)
	ROSAT HRI observations of the Local Group galaxies IC 10, NGC 147 and NGC 185.
o	WR 17, WR 18 are [MAC92] 17 and 18 in SIMBAD
o	<[BWF97] IC 10 X-1>. Table 1: <[BWF97] N> (Nos 1-5)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWH2003]
[BWH2003]	(Braatz+Wilson+Henkel+, 2003)
Write:	<<[BWH2003] BHHMMSS.s+DDMMSS>>
N:	58
Object:	H2O Maser (SIMBAD class: Maser)
Note:	N=58 H2O masers in 58 active galaxies.
Ref:	=2003ApJS..146..249B
by	BRAATZ J.A. , WILSON A.S., HENKEL C., GOUGH R., SINCLAIR M.
	Astrophys. J., Suppl. Ser., 146, 249-265 (2003)
	A survey for H_{2}O megamasers. III. Monitoring water vapor masers in active galaxies.
o	Table 2: <[BWH2003] BHHMMSS.s+DDMMSS> N=58.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWH2004]
[BWH2004]	(Belsole+Worrall+Hardcastle+, 2004)
Write:	<<[BWH2004] 3C 292 SN>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton and Chandra observations of 3C 292 field. S1 is most likely a background source, S2 strongly contaminates the extended emission of 3C 292.
Ref:	=2004MNRAS.352..924B
by	BELSOLE E. , WORRALL D.M., HARDCASTLE M.J., BIRKINSHAW M., LAWRENCE C.R.
	Mon. Not. R. Astron. Soc., 352, 924-938 (2004)
	XMM-Newton observations of three high-redshift radio galaxies.
o	Fig.6: <[BWH2004] 3C 292 SN> (Nos S1-S2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWH2007]
[BWH2007]	(Balogh+Wilman+Henderson+, 2007)
Write:	<<[BWH2007] NNN>>
N:	47
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	Galaxy groups selected from the CNOC2 redshift survey. About 20 fields were re-observed with the LDSS2 spectrograph on Magellan. See also [WBB2005].
Ref:	=2007MNRAS.374.1169B
by	BALOGH M.L. , WILMAN D., HENDERSON R.D.E., BOWER R.G., GILBANK D., WHITAKER R., MORRIS S.L., HAU G., MULCHAEY J.S., OEMLER A.Jr, CARLBERG R.G.
	Mon. Not. R. Astron. Soc., 374, 1169-1180 (2007)
	The stellar mass content of distant galaxy groups.
o	Table 1: <[BWH2007] NNN> N=47 among [Nos 1-366).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BWI
BWI	(Blanco, Window I)
Write:	<<BWI NNN>> <<BWI EN>>
N:	112+9
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	RR Lyrae (Nos 1-112) and (Nos E1-E9) E for Eclipsing. Identif. charts.
Ref:	=1992AJ....103.1872B
by	BLANCO B.M.
	Astron. J., 103, 1872-1927 (1992)
	RR Lyrae variables in a galactic bulge window.
o	<BWI NNN> N=112, <BWI EN> N=9
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [BWJ2017]
[BWJ2017]	(Beuther+Walsh+Johnston+, 2017)
Write:	<<[BWJ2017] N>>
N:	4
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA 690GHz observations of N=4 submillimeter cores in GAL 351.78-00.54.
in source:	GAL 351.78-00.54 = IRAS 17233-3606
Ref:	=2017A&A...603A..10B
by	BEUTHER H. , WALSH A.J., JOHNSTON K.G., HENNING T., KUIPER R., LONGMORE S.N., WALMSLEY C.M.
	Astron. Astrophys., 603A, 10-10 (2017)
	Fragmentation and disk formation in high-mass star formation: The ALMA view of G351.77-0.54 at 0.06'' resolution.
o	Fig. 3, Table 1: <[BWJ2017] N> (Nos 1-4).
o	Paragraph 3.2 : region OF1 not in SIMBAD.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWL2006]
[BWL2006]	(Boles+Winslow+Li+, 2006)
Write:	<<[BWL2006] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of SN 2006TE.
Ref:	=2006IAUC.8789....1B
by	BOLES T. , WINSLOW D., LI W., DUSZANOWICZ G., KLOEHR W., TRONDAL O., LUCKAS P., SCHWARTZ M., FRIEMAN J., MASI G., CORELLI P., KONSTANTINOS E.
	IAUC, 8789, 1 (2006)
	Supernovae 2006sr-2006te.
o	<[BWL2006] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWL2012]
[BWL2012]	(Blair+Winkler+Long, 2012)
Write:	<<[BWL2012] NNN>>
N:	271
Object:	Poss. SNR + [OIII] source (SIMBAD class: SNRemnant_Candidate = SuperNova Remnant Candidate)
Stat:	is completely incorporated in Simbad
Note:	Magellan 6.5m telescope IMACS observations of N=225 SNR candidates and N=46 [OIII]-selected nebulae in M83.
in source:	NGC 5236 = M 83
Ref:	=2012ApJS..203....8B
by	BLAIR W.P. , WINKLER P.F., LONG K.S.
	Astrophys. J., Suppl. Ser., 203, 8 (2012)
	The Magellan/IMACS catalog of optical supernova remnant candidates in M83.
o	(Erratum) erratum vol. 207, art. 40 (2013) and vol. 229, art. 43 (2017)
o	Table 2: <[BWL2012] NNN> (Nos 001-225, 301-346).
=E=	Catalogue in electronic form as J/ApJS/203/8
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWL2015]
[BWL2015]	(Blair+Winkler+Long+, 2015)
Write:	<<[BWL2015] B12-174a>>
N:	1
Object:	Poss. SNR (SIMBAD class: SNRemnant_Candidate = SuperNova Remnant Candidate)
Stat:	is completely incorporated in Simbad
Note:	Gemini South GMOS spectroscopic observations of N=1 very young remnant of a SN in M83. Use of archival HST WFC3 and X-ray Chandra images.
in source:	NGC 5236 = M 83
Ref:	=2015ApJ...800..118B
by	BLAIR W.P. , WINKLER P.F., LONG K.S., WHITMORE B.C., KIM H., SORIA R., KUNTZ K.D., PLUCINSKY P.P., DOPITA M.A., STOCKDALE C.
	Astrophys. J., 800, 118 (2015)
	A newly recognized very young supernova remnant in M83.
o	Figs. 1-2, 4-5: <[BWL2015] B12-174a> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWM2012]
[BWM2012]	(Brand+Wouterloot+Magnani, 2012) (Not yet in Simbad)
Write:	<<[BWM2012] HaNN>>
N:	10
Object:	Poss. Em* (SIMBAD class: Star)
Note:	TNG DOLORES observations of N=10 candidate Hα emission-line stars in the cloud MBM 18.
in source:	MBM 18 = LDN 1569
Ref:	=2012A&A...547A..85B
by	BRAND J. , WOUTERLOOT J.G.A., MAGNANI L.
	Astron. Astrophys., 547A, 85-85 (2012)
	Molecular gas and stars in the translucent cloud MBM 18 (LDN 1569).
o	Table 1: <[BWM2012] HaNN> (Nos Ha1-Ha10).
o	1WGA J043.0+0027 not found (misprint).
=E=	Catalogue in electronic form as J/A+A/547/A85
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWM94]
[BWM94]	(Bower+Wilson+Mulchaey+, 1994)
Write:	<<[BWM94] NGC 5929 A>>
N:	5
Object:	Cloud (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	PC HST observations. 1st ref.: Map in Fig. 2
in source:	NGC 5929
Ref:	=1994AJ....107.1686B
by	BOWER G.A. , WILSON A.S., MULCHAEY J.S., MILEY G.K., HECKMAN T.M., KROLIK J.H.
	Astron. J., 107, 1686-1694 (1994)
	Hubble Space Telescope images of the Seyfert galaxies NGC 5929 and MCG 8-11-11.
o	MCG 8-11-11 misprint for MCG -8-11-11. Components NE and SW in NGC 5929 = [WK89] NGC 5929 NE and SW
o	Fig.2: <[BWM94] NGC 5929 A> (Nos A-C)
Ref:	=1997A&A...328..493F
by	FERRUIT P. , PECONTAL E., WILSON A.S., BINETTE L.
	Astron. Astrophys., 328, 493-498 (1997)
	Sub-arcsecond resolution 2D (x,y,λ) spectrography of the emission line region of NGC 5929 with TIGER.
o	Components NE and SW in NGC 5929 = [WK89] NGC 5929 NE and SW
o	Table 2: <[BWM94] NGC 5929 A> (Nos D-E) added
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWS2002]
[BWS2002]	(Beuther+Walsh+Schilke+, 2002)
Write:	<<[BWS2002] JHHMMSS.s+DDMMSS.s>>
N:	26+43
Object:	CH3OH and H2O maser (SIMBAD class: Maser)
Note:	VLA and ATCA observations of N=26 CH3OH masers and N=43 H2O masers in 29 massive IRAS star-forming regions.
Ref:	=2002A&A...390..289B
by	BEUTHER H. , WALSH A., SCHILKE P., SRIDHARAN T.K., MENTEN K.M., WYROWSKI F.
	Astron. Astrophys., 390, 289-298 (2002)
	CH_{3}OH and H_{2}O masers in high-mass star-forming regions.
o	Table 2: <[BWS2002] JHHMMSS.s+DDMMSS.s> N=26+43.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWS2008]
[BWS2008]	(Blackburne+Wisotzki+Schechter, 2008)
Write:	<<[BWS2008] 1113-0641 A>> <<[BWS2008] a>>
N:	2+1+5
Object:	Grav. lensed image + G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Magellan 6.5m telescope, HST ACS and NICMOS observations of the lens system HE 1113-0641.
Ref:	=2008AJ....135..374B
by	BLACKBURNE J.A. , WISOTZKI L., SCHECHTER P.L.
	Astron. J., 135, 374-379 (2008)
	HE 1113-0641: the smallest-separation quadruple lens identified by a ground-based optical telescope.
o	Table 2, Fig.2: <[BWS2008] 1113-0641 A> (Nos A-D, G). Table 3, Fig.1: <[BWS2008] a> (Nos a-e).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWS2010]
[BWS2010]	(Bayliss+Wuyts+Sharon+, 2010)
Write:	<<[BWS2010] SDSS JHHMM+DDMM>>
N:	2
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Gemini North and APO 3.5m telescope observations of N=2 strongly lensing galaxy clusters.
Ref:	=2010ApJ...720.1559B
by	BAYLISS M.B. , WUYTS E., SHARON K., GLADDERS M.D., HENNAWI J.F., KOESTER B.P., DAHLE H.
	Astrophys. J., 720, 1559-1568 (2010)
	Two lensed lyman-α emitting galaxies at z~ 5.
o	<SGAS JHHMMSS+DDMMSS> N=2. <[BWS2010] SDSS JHHMM+DDMM> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BWSH
BWSH	(Barnes+Webster+Schmidt+Hughes)
Write:	<<BWSH BHHMMSS+DDMMSS>> <<BWSH WWN>>
N:	6
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=6 galaxies in the field of the lensing galaxy [Y88] G. 4 galaxies are new (format 'BHHMMSS+DDMMSS'), but the 6 have an alternative name (format 'WWN') given by the authors.
Ref:	=1999MNRAS.309..641B
by	BARNES D.G. , WEBSTER R.L., SCHMIDT R.W., HUGHES A.
	Mon. Not. R. Astron. Soc., 309, 641-650 (1999)
	Imaging HI in the lensing galaxy 2237+0305.
o	lensing galaxy 2237+0305 = [Y88] G
o	Table 1: <BWSH BHHMMSS+DDMMSS> = <BWSH WWN> (Nos C, S, SE, SW, NW1,NW2).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BWSS
BWSS	(Bolton+Westfold+Stanley +Slee)= (B1)
Write:	<<BWSS A>>
N:	10
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Ref:	=1954AuJPh...7...96B
by	BOLTON J.G. , WESTFOLD K.C., STANLEY G.J., SLEE O.B.
	Australian J. Phys., 7, 96-109 (1954)
	Galactic radiation at radio frequencies. VII. Discrete sources with large angular widths.
o	<BWSS A> (Nos A-J), No. I missing
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BWV2006]
[BWV2006]	(Boyer+Woodward+van Loon+, 2006)
Write:	<<[BWV2006] IRNa>>
N:	6
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Spitzer IRAC and MIPS observations of the Galactic globular cluster M15.
in source:	M 15 = NGC 7078
Ref:	=2006AJ....132.1415B
by	BOYER M.L. , WOODWARD C.E., VAN LOON J.T., GORDON K.D., EVANS A., GEHRZ R.D., HELTON L.A., POLOMSKI E.F.
	Astron. J., 132, 1415-1425 (2006)
	Stellar populations and mass loss in M15: a Spitzer space telescope detection of dust in the intracluster medium.
o	Fig. 1: <[BWV2006] IRNa> (Nos 1a-1b, 2, 3a-3b, 4). Table 3: <[BWV2006] SSTU JHHMMSS.ss+DDMMSS.s> N=2.
o	PN BB-1 = PN BoBn 1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWW2009]
[BWW2009]	(Browne+Welsh+Wheatley, 2009) (Not yet in Simbad)
Write:	<<[BWW2009] JHHMMSS.s+DDMMSS.s>>
N:	16
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	GALEX NUV and FUV observations of two fields in the Hyades and Pleiades open clusters.
in source:	Hyades = Cl Melotte 25
in source:	Pleiades = Cl Melotte 22
Ref:	=2009PASP..121..450B
by	BROWNE S.E. , WELSH B.Y., WHEATLEY J.
	PASP, 121, 450-460 (2009)
	GALEX ultraviolet observations of stellar variability in the Hyades and Pleiades clusters.
o	SDSS J0422842.78+171149.6 is a misprint for SDSS J042842.78+171149.6.
o	Table 1: <[BWW2009] JHHMMSS.s+DDMMSS.s> N=16.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BWW84]
[BWW84]	(Batrla+Walmsley+Wilson, 1984)
Write:	<<[BWW84] NN>>
N:	14
Object:	NH3 Cloud (SIMBAD class: Cloud)
Note:	Effelsberg 100m telescope observations. Search for NH3 clouds in Cas A.
in source:	NAME Cas A
Ref:	=1984A&A...136..127B
by	BATRLA W. , WALMSLEY C.M., WILSON T.L.
	Astron. Astrophys., 136, 127-132 (1984)
	Ammonia clouds in absorption against Cas A.
o	Table 1: <[BWW84] NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BX
BX	(BeppoSAX instrument)
*****	Avoid the usage of BX, prefer SAX
Origin	of the Acronym: L (1999A&A...352..532B)
Details on Acronym: BYB
BYB	(Baud+Young+Beichman+)= (B) = (Baud)
Write:	<<BYB NN>>
N:	70
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Rem:	identif. chart
in source:	NAME Cha Dark Cloud
Ref:	=1984ApJ...278L..53B
by	BAUD B. , YOUNG E., BEICHMAN C.A., BEINTEMA D.A., EMERSON J.P., HABING H.J., HARRIS S., JENNINGS R.E., MARSDEN P.L., WESSELIUS P.R.
	Astrophys. J., 278, 53-55 (1984)
	High-sensitivity IRAS observations of the Chamaeleon I dark cloud.
o	<BYB NN> (Nos 1-70)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BYB2017]
[BYB2017]	(Badescu+Yang+Bertoldi+, 2017)
Write:	<<[BYB2017] Bootes J1430+3522>> <<[BYB2017] JDDD.ddddd+DD.dddddd>>
N:	1+183
Object:	Overdensity + LAE (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	KPNO Mayall Mosaic narrowband observations of N=1 overdensity and N=183 Lyα emitters (LAEs) in the Bootes field (NDWFS).
in source:	NAME Bootes Field
Ref:	=2017ApJ...845..172B
by	BADESCU T. , YANG Y., BERTOLDI F., ZABLUDOFF A., KARIM A., MAGNELLI B.
	Astrophys. J., 845, 172-172 (2017)
	Discovery of a protocluster associated with a Lyα blob pair at z = 2.3.
o	<[BYB2017] Bootes J1430+3522> N=1. Table 1: <[BYB2017] JDDD.ddddd+DD.dddddd> N=183. Table 2: <[YZT2009] Blob N> (Nos 5-7) added.
=E=	Catalogue in electronic form as <J/ApJ/845/172/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BYF2011]
[BYF2011]	(Barnes+Yonekura+Fukui+, 2011)
Write:	<<[BYF2011] NNNa>>
N:	209+318+303
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat.	in SIMBAD: Table 1
Note:	NANTEN C18O observations of N=209 clouds. Follow-up observations in the HCO+ J=1->0 line with the Mopra 22m radio telescope.
Ref:	=2011ApJS..196...12B
by	BARNES P.J. , YONEKURA Y., FUKUI Y., MILLER A.T., MUHLEGGER M., AGARS L.C., MIYAMOTO Y., FURUKAWA N., PAPADOPOULOS G., JONES S.L., HERNANDEZ A.K., O'DOUGHERTY S.N., TAN J.C.
	Astrophys. J., Suppl. Ser., 196, 12 (2011)
	The Galactic Census of High- and Medium-mass Protostars. I. Catalogs and first results from Mopra HCO^+ maps.
o	Table 1: <[BYF2011] NNN> (Nos 1-209). Tables 4-5: <[BYF2011] NNNa> N=318+303 among (Nos 2-208b).
=E=	Catalogue in electronic form as <J/ApJS/196/12/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BYR98]
[BYR98]	(Bally+Yu+Rayner+, 1998) (Not yet in Simbad)
Write:	<<[BYR98] S106 Clump Na>>
N:	12
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Note:	HST WFPC2 observations
in source:	SH 2-106
Ref:	=1998AJ....116.1868B
by	BALLY J. , YU KA C., RAYNER J., ZINNECKER H.
	Astron. J., 116, 1868-1881 (1998)
	Hubble Space Telescope Wide Field Planetary Camera 2 observations of the young bipolar H II region S106.
o	Figs 4-6: <[BYR98] S106 Clump Na> (Nos 1-2, 3a-3b, 4a-4b, 5, 6a-6b, 7, 8a-8b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Byu
Byu	(Byurakan obs.)
*****	Avoid the usage of Byu, prefer [OSM2003]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BYY2014]
[BYY2014]	(Bai+Yee+Yan+, 2014)
Write:	<<[BYY2014] RCSJHHMM+DD BCG>> <<[BYY2014] RCSJHHMM+DDMM BCG>> <<[BYY2014] RXJHHMM+DD BCG>>
N:	29+8
Object:	BCG (SIMBAD class: BrightestCG = Brightest Galaxy in a Cluster (BCG))
Note:	N=29+8 brightest cluster galaxies (BCGs) with 0.3<z<0.9 selected from the first Red-sequence Cluster Survey and an X-ray cluster survey. Use of archival HST images.
Ref:	=2014ApJ...789..134B
by	BAI L. , YEE H.K.C., YAN R., LEE E., GILBANK D.G., ELLINGSON E., BARRIENTOS L.F., GLADDERS M.D., HSIEH B.C., LI I.H.
	Astrophys. J., 789, 134 (2014)
	The inside-out growth of the most massive galaxies at 0.3 < z < 0.9.
o	Table 1: <[BYY2014] RCSJHHMM+DD BCG> N=25, <[BYY2014] RCSJHHMM+DDMM BCG> N=4. Table 2: <[BYY2014] RXJHHMM+DD BCG> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BZ
BZ	(Brown+Zuckerman)
*****	Avoid the usage of BZ, prefer [BZ75]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BZ38]
[BZ38]	(Baade+Zwicky, 1938)
Write:	<<[BZ38] IC 4182 A>> <<[BZ38] IC 4182 a>> <<[BZ38] NGC 1003 A>> <<[BZ38] NGC 1003 a>>
N:	1+25+1+21
Object:	* (SIMBAD class: Star)
Note:	Comparison stars in the field of IC 4182 and NGC 1003.
Ref:	=1938ApJ....88..411B
by	BAADE W. , ZWICKY F.
	Astrophys. J., 88, 411-421 (1938)
	Photographic light-curves of the two supernovae in IC 4182 and NGC 1003.
o	The two supernovae = SN 1937C and SN 1937D.
o	Table 1: <[BZ38] IC 4182 A> (No. A), <[BZ38] IC 4182 a> (Nos a-y). Table 3: <[BZ38] NGC 1003 A> (No. A), <[BZ38] NGC 1003 a> (Nos a-u).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BZ75]
[BZ75]	(Brown+Zuckerman, 1975)= (BZ)
Write:	<<[BZ75] Oph N>> <<[BZ75] R CrA N>>
N:	6+2
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	HII in Ophiuchus DCld, format 'Oph N', N=6 HII in R CrA DCld, format 'R CrA N', N=2
in source:	NAME rho Oph Cloud
in source:	NAME R CrA Cloud
Ref:	=1975ApJ...202L.125B
by	BROWN R.L. , ZUCKERMAN B.
	Astrophys. J., 202, 125-128 (1975)
	Compact H II regions in the Ophiuchus and R Coronae Austrinae dark clouds.
o	<[BZ75] Oph N> N=6, <[BZ75] R CrA N> N=2
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [BZ91]
[BZ91]	(Baath+Zhang, 1991)
Write:	<<[BZ91] 0735+178 AN>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio components of QSO 0735+178. See also Gabuzda, [GMA99b].
in source:	QSO B0735+178
Ref:	=1991A&A...243..328B
by	BAATH L.B. , ZHANG F.J.
	Astron. Astrophys., 243, 328-None (1991)
	The radio fine structure of the BL Lacertae object 0735+178.
o	Fig.1: <[BZ91] 0735+178 AN> (Nos A, B, C0, C1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BZA2000]
[BZA2000]	(Brandner+Zinnecker+Alcala+, 2000) (Not yet in Simbad)
Write:	<<[BZA2000] RX JHHMM.m+DDMM a>> <<[BZA2000] RX JHHMM.m+DDMMB a>>
N:	12+5
Object:	* in ** (SIMBAD class: Star)
Note:	Table 4: 6 TTau* (RX J counterparts) are binaries with 2 components 'a' and 'b'. 5 TTau* have a companion 'c'.
Ref:	=2000AJ....120..950B
by	BRANDNER W. , ZINNECKER H., ALCALA J.M., ALLARD F., COVINO E., FRINK S., KOEHLER R., KUNKEL M., MONETI A., SCHWEITZER A.
	Astron. J., 120, 950-962 (2000)
	Timescales of disk evolution and planet formation: HST, adaptive optics, and ISO observations of weak-line and post-T Tauri stars.
o	Table 4: <[BZA2000] RX JHHMM.m+DDMM a>, <[BZA2000] RX JHHMM.m+DDMMA a>, N=12+5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BZB2001]
[BZB2001]	(Bardelli+Zucca+Baldi, 2001)
Write:	<<[BZB2001] JHHMMSS.ss+DDMMSS.s>>
N:	581
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
in source:	Shapley Concentration:ACO 3528 = ACO 3528
Ref:	=2001MNRAS.320..387B
by	BARDELLI S. , ZUCCA E., BALDI A.
	Mon. Not. R. Astron. Soc., 320, 387-400 (2001)
	A study of the core of the Shapley Concentration - V. The A3528 complex: a young merger event?
o	Table 2: <[BZB2001] JHHMMSS.ss+DDMMSS.s> N=581.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BZB2004]
[BZB2004]	(Blakeslee+Zwkser+Benitez+, 2004)
Write:	<<[BZB2004] JHHMMSS+DDMMSS>> <<[BZB2004] Main Arc>> <<[BZB2004] Knot NN>>
N:	1+1+10
Object:	G + Arc (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST ACS images in a parallel field during NICMOS HST Ultra Deep Field observations. Images of a lensing galaxy and the lensed arc (Main Arc) composed of 10 bright knots.
Ref:	=2004ApJ...602L...9B
by	BLAKESLEE J.P. , ZEKSER K.C., BENITEZ N., FRANX M., WHITE R.L., FORD H.C., BOUWENS R.J., INFANTE L., CROSS N.J., HERTLING G., HOLDEN B.P., ILLINGWORTH G.D., MOTTA V., MENANTEAU F., MEURER G.R., POSTMAN M., ROSATI P., ZHENG W.
	Astrophys. J., 602, 9-12 (2004)
	Advanced camera for surveys observations of a strongly lensed arc in a field elliptical galaxy.
o	Table 1: <[BZB2004] JHHMMSS+DDMMSS> N=1. Fig.2: <[BZB2004] Main Arc> N=1, <[BZB2004] Knot NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BZB2007]
[BZB2007]	(Beuther Zhang+Bergin+, 2007)
Write:	<<[BZB2007] submmN>>
N:	6
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	Submillimeter Array (SMA) observations of the hot core associated with the HII region [WC89] 029.96-0.02.
in source:	[WC89] 029.96-0.02
Ref:	=2007A&A...468.1045B
by	BEUTHER H. , ZHANG Q., BERGIN E.A., SRIDHARAN T.K., HUNTER T.R., LEURINI S.
	Astron. Astrophys., 468, 1045-1056 (2007)
	Dust and gas emission in the prototypical hot core G29.96-0.02 at sub-arcsecond resolution.
o	Fig.1, Table 2: <[BZB2007] submmN> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BZB2012]
[BZB2012]	(Bonfini+zezas +? Birkinshaw+, 2012)
Write:	<<[BZB2012] NNN>>
N:	718
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	HST WFPC2 observations of N=718 globular cluster candidates in NGC 4261.
in source:	NGC 4261
Ref:	=2012MNRAS.421.2872B
by	BONFINI P. , ZEZAS A., BIRKINSHAW M., WORRALL D.M., FABBIANO G., O'SULLIVAN E., TRINCHIERI G., WOLTER A.
	Mon. Not. R. Astron. Soc., 421, 2872-2887 (2012)
	Studying the asymmetry of the globular cluster population of NGC 4261.
o	Table 3: <[BZB2012] NNN> (Nos 1-718).
=E=	Catalogue in electronic form as J/MNRAS/421/2872
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BZC97]
[BZC97]	(Belloni+Zampieri+Campana, 1997)
Write:	<<[BZC97] Rift-N>> <<[BZC97] OB7-N>>
N:	2+2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations
in source:	NAME Cyg Rift
in source:	NAME ASS CYG OB 7-
Ref:	=1997A&A...319..525B
by	BELLONI T. , ZAMPIERI L., CAMPANA S.
	Astron. Astrophys., 319, 525-534 (1997)
	Search for old neutron stars in molecular clouds: Cygnus rift and Cygnus OB7.
o	Table 5: <[BZC97] Rift-N> (Nos 1-2), <[BZC97] OB7-N> (Nos 1-2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BZG2004]
[BZG2004]	(Beuther+Zhang+Greenhill+, 2004)
Write:	<<[BZG2004] SMA1>>
N:	1
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SMA 865µm observations of N=1 submillimter source in the Orion KL region.
in source:	NAME Orion KL
Ref:	=2004ApJ...616L..31B
by	BEUTHER H. , ZHANG Q., GREENHILL L.J., REID M.J., WILNER D., KETO E., MARRONE D., HO P.T.P., MORAN J.M., RAO R., SHINNAGA H., LIU S.-Y.
	Astrophys. J., 616, 31-34 (2004)
	Subarcsecond submillimeter continuum observations of Orion KL.
o	Fig. 1, Table 1: <[BZG2004] SMA1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BZH2007]
[BZH2007]	(Beuther+Zhang+Hunter+, 2007)
Write:	<<[BZH2007] Peak N>>
N:	2
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	Submillimeter Array observations of IRAS 23151+5912.
in source:	IRAS 23151+5912
Ref:	=2007A&A...473..493B
by	BEUTHER H. , ZHANG Q., HUNTER T.R., SRIDHARAN T.K., BERGIN E.A.
	Astron. Astrophys., 473, 493-500 (2007)
	The 10^{5} L_☉ high-mass protostellar object IRAS23151+5912.
o	Table 2, Fig.1: <[BZH2007] Peak N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: BzK
BzK	(B, z, and K band preselected) (Not yet in Simbad)
*****	Avoid the usage of BzK, prefer [HMS2009]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BzK
BzK	(B, z, and K band preselected)
*****	Avoid the usage of BzK, prefer [DDO2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: BzK
BzK	(B, z, and K-band photometry)
*****	Avoid the usage of BzK, prefer [LSE2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [BZM96]
[BZM96]	(Bardelli+Zucca+Malizia+, 1996)
Write:	<<[BZM96] NN>>
N:	22
Object:	(X) in ClG (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations. fig.2: map See also [BZV94] and [BZZ98].
in source:	NAME ACO 3558 Complex
Ref:	=1996A&A...305..435B
by	BARDELLI S. , ZUCCA E., MALIZIA A., ZAMORANI G., SCARAMELLA R., VETTOLANI G.
	Astron. Astrophys., 305, 435-449 (1996)
	A study of the core of the Shapley concentration. II. ROSAT observation of A 3558.
o	Table 3: <[BZM96] NN> (Nos 1-22)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BZO2009]
[BZO2009]	(Barbuy+Zoccali+Ortolani+, 2009)
Write:	<<[BZO2009] A-NNN>>
N:	9
Object:	* (SIMBAD class: Star)
Note:	VLT FLAMES+GIRAFFE observations of NGC 6522. The star IDs are adopted according to the fact that FLAMES+GIRAFFE has provided spectra for 134 stars in each of the bright (B) and faint (F) stars selected in the field. See also [ZHL2008].
in source:	NGC 6522
Ref:	=2009A&A...507..405B
by	BARBUY B. , ZOCCALI M., ORTOLANI S., HILL V., MINNITI D., BICA E., RENZINI A., GOMEZ A.
	Astron. Astrophys., 507, 405-415 (2009)
	VLT-FLAMES analysis of 8 giants in the bulge metal-poor globular cluster NGC 6522: oldest cluster in the Galaxy? Analysis of 8 giants in NGC 6522.
o	Tables 2-4: <[BZO2009] A-NNN> N=9.
Details on Acronym: [BZR2006]
[BZR2006]	(Bergond+Zepf+Romanowsky+, 2006)
Write:	<<[BZR2006] gcNNNN>> <<[BZR2006] adNNNN>>
N:	102+6
Object:	Poss. GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	VLT-FLAMES observations around the Leo I group of galaxies. Search for globular clusters from an unpublished list of Rhode and Zepf (2004AJ....127..302R).
in source:	NAME LEO I GROUP = NAME M 96 GROUP
Ref:	=2006A&A...448..155B
by	BERGOND G. , ZEPF S.E., ROMANOWSKY A.J., SHARPLES R.M., RHODE K.L.
	Astron. Astrophys., 448, 155-164 (2006)
	Wide-field kinematics of globular clusters in the Leo I group.
o	(Erratum) erratum vol. 618, art. C5 (2018)
o	Tables A1, A2, A3: <[BZR2006] gcNNNN> N=102 among (Nos gc139 to gc1272), <[BZR2006] adNNNN> N=6 among (Nos ad411 to ad1481).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BZR2011]
[BZR2011]	(Bejar+Zapatero Osorio+Rebolo+, 2011)= (S Ori)
Write:	<<[BZR2011] S Ori JHHMMSS.ss+DDMMSS.s>>
N:	154
Object:	* (SIMBAD class: Star)
Note:	INT WFC (optical) and TCS CAIN (NIR), and Calar Alto telescope MAGIC (NIR) photometry of the σ Orionis star cluster. Use of 2MASS and UKIDSS data. See also [BMZ2001], [BZR99].
in source:	NAME sig Ori Cluster
Ref:	=2011ApJ...743...64B
by	BEJAR V.J.S. , ZAPATERO OSORIO M.R., REBOLO R., CABALLERO J.A., BARRADO D., MARTIN E.L., MUNDT R., BAILER-JONES C.A.L.
	Astrophys. J., 743, 64 (2011)
	The substellar population of σ Orionis: a deep wide survey.
o	Tables 2-3: <[BZR2011] S Ori JHHMMSS.ss+DDMMSS.s> N=154.
=E=	Catalogue in electronic form as J/ApJ/743/64
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BZR2017]
[BZR2017]	(Bayliss+Zengo+Ruel+, 2017)
Write:	<<[BZR2017] JHHMMSS.ss+DDMMSS.s>>
N:	1905
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Gemini South GMOS and Magellan Baade telescope IMACS spectroscopic observations of N=1905 galaxies associated with N=89 galaxy clusters detected in the SPT-SZ and ACT-SZ surveys. See also [RBB2014] and [BRS2016].
Ref:	=2017ApJ...837...88B
by	BAYLISS M.B. , ZENGO K., RUEL J., BENSON B.A., BLEEM L.E., BOCQUET S., BULBUL E., BRODWIN M., CAPASSO R., CHIU I.-N., McDONALD M., RAPETTI D., SARO A., STALDER B., STARK A.A., STRAZZULLO V., STUBBS C.W., ZENTENO A.
	Astrophys. J., 837, 88-88 (2017)
	Velocity segregation and systematic biases in velocity dispersion estimates with the SPT-GMOS spectroscopic survey.
o	Table 1: <[BZR2017] JHHMMSS.ss+DDMMSS.s> N=1905.
=E=	Catalogue in electronic form as J/ApJ/837/88
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BZR99]
[BZR99]	(Bejar+Zapatero Osorio+Rebolo, 1999)= (S Ori)
Write:	<<[BZR99] S Ori NN>>
N:	74
Object:	Poss. * in Cl* (SIMBAD class: Star)
Note:	Candidate star members of Sigma Orionis Cluster. Nos 59 and 63 missing. See also [BMZ2001]. Finding charts.
in source:	NAME sig Ori Cluster
Ref:	=1999ApJ...521..671B
by	BEJAR V.J.S. , ZAPATERO OSORIO M.R., REBOLO R.
	Astrophys. J., 521, 671-681 (1999)
	A search for very low mass stars and brown dwarfs in the young σ Orionis cluster.
o	Tables 2, 3: <[BZR99] S Ori NN> (Nos 1-49).
Ref:	=2000Sci...290..103Z
by	ZAPATERO OSORIO M.R. , BEJAR V.J.S., MARTIN E.L., REBOLO R., BARRADO Y NAVASCUES D., BAILER-JONES C.A.L., MUNDT R.
	Science, 290, 103-107 (2000)
	Discovery of young, isolated planetary mass objects in the σ Orionis star cluster.
o	Table 1, col(1): <[BZR99] S Ori NN> (Nos 50-69, 59 and 63 missing). Table 1, col(2): <[BMZ2001] S Ori JHHMMSS.s+DDMMSS> N=19 added.
Ref:	=2002ApJ...578..536Z
by	ZAPATERO OSORIO M.R. , BEJAR V.J.S., MARTIN E.L., REBOLO R., BARRADO Y NAVASCUES D., MUNDT R., EISLOEFFEL J., CABALLERO J.A.
	Astrophys. J., 578, 536-542 (2002)
	A methane, isolated, planetary-mass object in Orion.
o	<[BZR99] S Ori NN> (No. 70) added. <[BMZ2001] S Ori JHHMMSS.s+DDMMSS> N=1 added.
Ref:	=2002A&A...393L..85B
by	BARRADO Y NAVASCUES D. , ZAPATERO OSORIO M.R., MARTIN E.L., BEJAR V.J.S., REBOLO R., MUNDT R.
	Astron. Astrophys., 393, 85-88 (2002)
	Discovery of a very cool object with extraordinarily strong Hα emission.
o	PC 0025+0047 is a misprint for PC 0025+0447.
o	<[BZR99] S Ori NN> (No. 71) added. <[BMZ2001] S Ori JHHMMSS.s+DDMMSS> N=1 added.
Ref:	=2009A&A...506.1169B
by	BIHAIN G. , REBOLO R., ZAPATERO OSORIO M.R., BEJAR V.J.S., VILLO-PEREZ I., DIAZ-SANCHEZ A., PEREZ-GARRIDO A., CABALLERO J.A., BAILER-JONES C.A.L., BARRADO Y NAVASCUES D., EISLOEFFEL J., FORVEILLE T., GOLDMAN B., HENNING T., MARTIN E.L., MUNDT R.
	Astron. Astrophys., 506, 1169-1182 (2009)
	Candidate free-floating super-Jupiters in the young σ Orionis open cluster.
o	Table 4: <[BZR99] S Ori NN> (Nos 72-74) added. Table 5: <[BMZ2001] S Ori JHHMMSS.s+DDMMSS> N=2 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BZV94]
[BZV94]	(Bardelli+Zucca+Vettolani+, 1994)
Write:	<<[BZV94] F-NNN>>
N:	383
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Table 2: G in fields (Nos 2-9). See also [BZM96] and [BZZ98].
in source:	NAME Shapley Supercluster = NAME Shapley Concentration
Ref:	=1994MNRAS.267..665B
by	BARDELLI S. , ZUCCA E., VETTOLANI G., ZAMORANI G., SCARAMELLA R., COLLINS C.A., MacGILLIVRAY H.T.
	Mon. Not. R. Astron. Soc., 267, 665-691 (1994)
	A study of the core of the Shapley concentration - I. The sample.
o	Table 2: <[BZV94] F-NNN> N=383
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BZZ2000]
[BZZ2000]	(Bardelli+Zucca+Zamorani+, 2000)
Write:	<<[BZZ2000] JHHMMSS.ss+DDMMSS.s>>
N:	442
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Redshift survey of intercluster galaxies in the central region of the Shapley Concentration supercluster.
in source:	NAME Shapley Supercluster = NAME Shapley Concentration
Ref:	=2000MNRAS.312..540B
by	BARDELLI S. , ZUCCA E., ZAMORANI G., MOSCARDINI L., SCARAMELLA R.
	Mon. Not. R. Astron. Soc., 312, 540-556 (2000)
	A study of the core of the Shapley Concentration - IV. Distribution of intercluster galaxies and supercluster properties.
o	Table 2: <[BZZ2000] JHHMMSS.ss-DDMMSS.s> N=442.
=E=	Catalogue in electronic form as J/MNRAS/312/540
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [BZZ98]
[BZZ98]	(Bardelli+Zucca+Zamorani+, 1998)
Write:	<<[BZZ98] F-NN>>
N:	214
Object:	G (SIMBAD class: Galaxy)
Note:	Table 2: G in 5 fields (Nos 1-5). Among the 214 objects, 40 are stars. See also [BZV94] and [BZZ98].
in source:	NAME ACO 3558 Complex
Ref:	=1998MNRAS.296..599B
by	BARDELLI S. , ZUCCA E., ZAMORANI G., VETTOLANI G., SCARAMELLA R.
	Mon. Not. R. Astron. Soc., 296, 599-613 (1998)
	A study of the core of the Shapley concentration - III. Properties of the clusters in the A3558 complex.
o	Table 2: <[BZZ98] 1-NN> (Nos 1-40), <[BZZ98] 2-NN> (Nos 1-43), <[BZZ98] 3-NN> (Nos 1-42), <[BZZ98] 4-NN> (Nos 1-44), <[BZZ98] 5-NN> (Nos 1-45).
=E=	Catalogue in electronic form as J/MNRAS/296/599
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: C
C	(Cluster) (Not yet in Simbad)
Write:	<<C MMSSDDMMm>>
N:	113+15
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	Format where the hours (00h) and the declination sign (+) are omitted. Use the 2nd col. format 'NNN', Bol in 1st ref., ACH in 2nd ref.
in source:	M 31 = NGC 224
Ref:	=1987A&AS...67..447B
by	BATTISTINI P. , BONOLI F., BRACCESI A., FEDERICI L., FUSI PECCI F., MARANO B., BOERNGEN F.
	Astron. Astrophys., Suppl. Ser., 67, 447-482 (1987)
	Search for (globular) clusters in M 31. IV. Candidates in a 3x3° square field centered on M 31.
o	Table IV, col(1): The ID CMMSSDDMMm is not used in SIMBAD.
o	Table IV, col(1): <C MMSSDDMMm> N=113. Tables IV, V: <Bol NNN> (Nos 289-513, Nos 334 and 359 missing). Table VI: <Bol DNNN> (Nos D133-D350).
Ref:	=1992A&A...256...95A
by	AURIERE M. , COUPINOT G., HECQUET J.
	Astron. Astrophys., 256, 95-103 (1992)
	New globular clusters in the bulge of M 31.
o	Tables 2,3, col(1): The ID CMMSSDDMMm is not used in SIMBAD.
o	Tables 2,3, col(1): <C MMSSDDMMm> N=34. Tables 3, 4, col(2),(1): <ACH NN> (Nos 1-15).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: C
C	(Caldwell) (Not yet in Simbad)
*****	Avoid the usage of C, prefer Caldwell
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: C
C	(Complementary)
*****	Avoid the usage of C, prefer Ardb
Details on Acronym: C
C	(Cluster)
Write:	<<C HHMM+DDd>> <<C JHHMM+DDd>>
Object:	OCl + GCl (SIMBAD class: Cluster* = Cluster of Stars)
Note:	1979: Catalogue of open cluster data, 1st edition, Lynga, Lund Observatory. 1987: Catalogue of Open Cluster Data, 5th edition, Lynga, Lund Observatory. Format 'JHHMM+DDd' appears for the 1st time in 1996AJ....112.2013S
Auth.:	LYNGA G.
Ref:	=1982BICDS..23...89L
by	LYNGA G.
	Bull. Inf. Centre Donnees Stellaires, 23, 89-None (1982)
	IAU numbers for some recently discovered clusters.
o	<C HHMM+DDd> N=13
Ref:	=1983BICDS..24..127L
by	LYNGA G.
	Bull. Inf. Centre Donnees Stellaires, 24, 127-127 (1983)
	IAU Commission No. 37: IAU numbers for some recently discovered clusters.
o	<C HHMM+DDd> N=6
Ref:	=1996AJ....112.2013S
by	SARAJEDINI A. , GEISLER D.
	Astron. J., 112, 2013-None (1996)
	Deep photometry of the outer halo globular cluster in Pyxis.
o	<C J0908-373>. Table 1: <[SG96b] NNN> N=?
=E=	Catalogue in electronic form as VII/92
=E=	Catalogue in electronic form as VII/151
=E=	Catalogue in electronic form as VII/229
Details on Acronym: C
C	(Cristiani)
*****	Avoid the usage of C, prefer [C87]
Origin	of the Acronym: L (1990ApJ...351..377Y)
Details on Acronym: C
C	(Cambridge survey)
*****	Avoid the usage of C, prefer Cambridge
Origin	of the Acronym: L (1997MNRAS.288...78T)
Details on Acronym: C
C	(Case univ.)
*****	Avoid the usage of C, prefer Case
Details on Acronym: C
C	(Ciardullo+)
*****	Avoid the usage of C, prefer [CFN87]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: C
C	(Charon occult.)
*****	Avoid the usage of C, prefer Charon
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: C
C	(Cincinnati obs.)
*****	Avoid the usage of C, prefer Ci
Details on Acronym: C
C	(Cluster of G)
*****	Avoid the usage of C, prefer ClG
Details on Acronym: C
C	(Calzetti+)
*****	Avoid the usage of C, prefer [CMB97]
Origin	of the Acronym: L (1998AJ....116.1212T)
Details on Acronym: C
C	(Cristiani+)
*****	Avoid the usage of C, prefer [CVV84]
Origin	of the Acronym: L (Veron)
Details on Acronym: C
C	(Cloud Complex labelled C)
*****	Avoid the usage of C, prefer [GVC73]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: C
C	(Cloud Complex labelled C)
Note:	HVC Complex C
*****	Avoid the usage of C, prefer [H68]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: C
C	(Cluster)
*****	Avoid the usage of C, prefer [H75]
Origin	of the Acronym: L (1999AJ....117..238B)
Details on Acronym: C
C	(Chamaeleon)
*****	Avoid the usage of C, prefer HJM
Origin	of the Acronym: L (1991MNRAS.251..303P)
Details on Acronym: C
C	(Case univ.)
*****	Avoid the usage of C, prefer Case
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: C
C	(Cluster)
*****	Avoid the usage of C, prefer SKHB
Origin	of the Acronym: L = Found in the literature
Details on Acronym: C
C	(Calar Alto Deep Imaging Survey)
*****	Avoid the usage of C, prefer [TBF99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 7C(G)
7C(G)	(7th Cambridge catalog, Galactic plane)
*****	Avoid the usage of 7C(G), prefer 7C
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 4C(T)
4C(T)	(4th Cambridge catalog, Total flux)
*****	Avoid the usage of 4C(T), prefer 4CT
Details on Acronym: C*
C*	(Carbon *)
*****	Avoid the usage of C*, prefer [BEM91]
Origin	of the Acronym: L (1998MNRAS.294....1T)
Details on Acronym: C*
C*	(Cool Carbon *)= CCS = (CNUM) = CStars = (Stephenson) = (Stf)
Write:	<<C* NNNN>>
N:	3324
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Note:	Catalog: (Nos 1-3219). (Nos 3220-3324) are numbered by us (ref. 1985AJ.....90..784S), and also found in the literature as NC NNN (Nos 1-105) Updated by the comprehensive catalogue CGCS (ref. 1989PW&SO...3b...1S)
Ref:	=1973PW&SO...1d...1S
by	STEPHENSON C.B.
	Publ. Warner & Swasey Obs., 1, part no 4, 1-79 (1973)
	A general catalogue of cool carbon stars.
o	<C* NNNN> (Nos 1-3219)
Ref:	=1985AJ.....90..784S
by	STEPHENSON C.B.
	Astron. J., 90, 784-786 (1985)
	New carbon stars found in a hemispheric survey.
o	<C* NNNN> (Nos 3220-3324) = <NAME NC NNN> (Nos 1-105). Unnumbered by the author
Details on Acronym: 6C**
6C**	(6th Cambridge catalog, new sample)
Write:	<<6C** HHMM+DDMM>>
N:	68
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	New sample of radio sources drawn from the 151MHz 6C survey, filtered to find radio galaxies at z>4.
Ref:	=2006MNRAS.373.1531C
by	CRUZ M.J. , JARVIS M.J., BLUNDELL K.M., RAWLINGS S., CROFT S., KLOCKNER H.-R., McLURE R.J., SIMPSON C., TARGETT T.A., WILLOTT C.J.
	Mon. Not. R. Astron. Soc., 373, 1531-1562 (2006)
	The 6C* sample of steep-spectrum radio sources - I. Radio data,* near-infrared imaging and optical spectroscopy.
o	Table 2: <6C** HHMM+DDMM> N=68.
=E=	Catalogue in electronic form as J/MNRAS/373/1531
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 6C*
6C*	(Blundell+Rawlings+Eales+, 1998)
Write:	<<6C* HHMM+DDd>>
N:	34
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Sample of steep spectrum radio sources from the 6C survey, designed to find radio galaxies at z>4.
Ref:	=1998MNRAS.295..265B
by	BLUNDELL K.M. , RAWLINGS S., EALES S.A., TAYLOR G.B., BRADLEY A.D.
	Mon. Not. R. Astron. Soc., 295, 265-279 (1998)
	A sample of 6C radio sources designed to find objects at redshift z>4. I. The radio data.
o	Table 1: <6C* HHMM+DDd> N=34.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: C-S
C-S	(Cohen+Schwartz)
N:	1
Object:	* near HH (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	The 1st star in table 1, supposed to excite HH1, has been studied by Cohen+Schwartz 1979, Ap. J. Lett. 233, L77-L80 and plate 2, and by Mundt+Hartman 1983, Ap. J. 268, 766-777, and is named the Cohen-Schwartz star (C-S).
Ref:	=1980MNRAS.191..165C
by	COHEN M. , SCHWARTZ R.D.
	Mon. Not. R. Astron. Soc., 191, 165-168 (1980)
	A search for the exciting stars of Herbig-Haro objects.
o	Table 1, 1st star: <NAME C-S>
Origin	of the Acronym: L = Found in the literature
Details on Acronym: C07
C07	(Clark+, 2007)
*****	Avoid the usage of C07, prefer [CMN2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 1C
1C	(1st Cambridge catalog)= (Ryle)
Write:	<<1C HH.NN>>
N:	50
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1950MNRAS.110..508R
by	RYLE M. , SMITH F.G., ELSMORE B.
	Mon. Not. R. Astron. Soc., 110, 508-None (1950)
	A preliminary survey of the radio stars in the northern hemisphere.
o	Table I: <1C HH.NN> N=50
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 10C
10C	(10th Cambridge catalog)
Write:	<<10C JHHMMSS+DDMMSS>>
N:	1897
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	The 10th Cambridge Survey of Radio Sources contains N=1897 sources, observed with the AMI (Arcminute Microkelvin Imager) Large Array at 15.7GHz.
Ref:	=2011MNRAS.415.2708D
by	DAVIES M.L. , FRANZEN T.M.O., WALDRAM E.M., GRAINGE K.J.B., HOBSON M.P., HURLEY-WALKER N., LASENBY A., OLAMAIE M., POOLEY G.G., RILEY J.M., RODRIGUEZ-GONZALVEZ C., SAUNDERS R.D.E., SCAIFE A.M.M., SCHAMMEL M.P., SCOTT P.F., SHIMWELL T.W., TITTERINGTON D.J., ZWART J.T.L.
	Mon. Not. R. Astron. Soc., 415, 2708-2722 (2011)
	10C survey of radio sources at 15.7 GHz – II. First results.
o	Table 1: <10C JHHMMSS+DDMMSS> N=1897.
=E=	Catalogue in electronic form as J/MNRAS/415/2708
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 4C1
4C1	(4th Cambridge catalog)
*****	Avoid the usage of 4C1, prefer 4C
Details on Acronym: 2C
2C	(2nd Cambridge catalog)
Write:	<<2C NNNN>>
N:	1936
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1955MmRAS..67..106S
by	SHAKESHAFT J.R. , RYLE M., BALDWIN J.E., ELSMORE B., THOMSON J.H.
	Mem. R. Astron. Soc., 67, 106-154 (1955)
	A survey of radio sources between declinations -38 and +83.
o	<2C NNNN> (Nos 1-1936)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [C2000]
[C2000]	(Clements, 2000)= ([C2000a]) (Not yet in Simbad)
Write:	<<[C2000] RN>>
N:	5
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=5 red companions (Nos R1-R5) in the field of the QSO 1550-269.
Ref:	=2000MNRAS.312L..61C
by	CLEMENTS D.L.
	Mon. Not. R. Astron. Soc., 312, 61-64 (2000)
	Red companions to a z=2.15 radio-loud quasar.
o	Fig.1, Table 1: <[C2000] AN> (Nos R1-R5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2000a]
[C2000a]	(Clements, 2000) (Not yet in Simbad)
*****	Avoid the usage of [C2000a], prefer [C2000]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2000b]
[C2000b]	(Carpenter, 2000)
Write:	<<[C2000b] NN>>
N:	14
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	From 2MASS PSC, second incremental release. No. 1 is in Per region, (Nos 2-8) are in Ori A, (Nos 9-10) are in Ori B, (Nos 11-14) are in Mon R2.
in source:	NAME Per Region
in source:	NAME Ori A
in source:	NAME Ori B
in source:	NAME Mon R2 GMC
Ref:	=2000AJ....120.3139C
by	CARPENTER J.M.
	Astron. J., 120, 3139-3161 (2000)
	2MASS observations of the Perseus, Orion A, Orion B, and Monoceros R2 molecular clouds.
o	Table 2: <[C2000b] NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2001]
[C2001]	(Comeron, 2001)= ([C2001a])
Write:	<<[C2001] NN>>
N:	40
Object:	Star (SIMBAD class: Association = Association of Stars)
Note:	VLT archive observations of M 83 are used to study a complex in the disk of that galaxy that shows a remarkable similarity to the Gould Belt. Finding chart in Fig.4.
in source:	M 83 = NGC 5236
Ref:	=2001A&A...365..417C
by	COMERON F.
	Astron. Astrophys., 365, 417-423 (2001)
	A Gould-Belt-like structure in M 83.
o	Table 1: <[C2001] NN> (Nos 1-40).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2001a]
[C2001a]	(Comeron, 2001)
*****	Avoid the usage of [C2001a], prefer [C2001]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2001b]
[C2001b]	(Cohen, 2001)
Write:	<<[C2001b] JHHMMSS.ss+DDMMSS.s>>
N:	519+47+2
Object:	G (SIMBAD class: Galaxy)
Note:	See also [CHB2000], [HPA2000].
in source:	NAME HDFN
Ref:	=2001AJ....121.2895C
by	COHEN J.G.
	Astron. J., 121, 2895-2914 (2001)
	Caltech faint galaxy redshift survey. XIII. Spectral energy distributions for galaxies in the region of the Hubble Deep Field North.
o	Tables 6A, 6B: [CHB2000] FMMSS.ss-MMSS.s and [CHB2000] HMMSS.ss-MMSS.s, galaxies with additional redshifts.
o	Tables 1, 7A, 7B: <[C2001b] JHHMMSS.ss+DDMMSS.s> N=519+47+2.
=E=	Catalogue in electronic form as J/AJ/121/2895
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2001c]
[C2001c]	(Cseresnjes, 2001)
Write:	<<[C2001c] vdNNfNNN>> <<[C2001c] vsNNfNNN>>
N:	66
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Stat:	is completely incorporated in Simbad
Note:	RR Lyrae in Sgr dwarf galaxy (N=45) and in the Galaxy (N=21). In the format, the first letter 'v' stands for variable star, the second letter 'd' or 's' for one of the 2 plates 'DUO' and 'SAG', each plate is divided in 28x28 parts 'NNN', and in each part a star has a numbering 'NN'. Finding charts Fig.4.
in source:	NAME SDG = NAME Sgr Dwarf Galaxy
Ref:	=2001A&A...375..909C
by	CSERESNJES P.
	Astron. Astrophys., 375, 909-921 (2001)
	RR Lyrae stars in the Sagittarius dwarf galaxy: Period analysis.
o	Table 15: misprint for Table 5.
o	Tables 1-4: <[C2001c] vdNNfNNN>, <[C2001c] vsNNfNNN>, N=66.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2001d]
[C2001d]	(Churchill, 2001)
Write:	<<[C2001d] QSO JHHMM+DDMM abs N.NNNN>>
N:	4
Object:	Absorber
Note:	HST observations with the Faint Object Spectrograph of MgII absorption lines in 4 QSOs.
Ref:	=2001ApJ...560...92C
by	CHURCHILL C.W.
	Astrophys. J., 560, 92-100 (2001)
	Mg II absorber number density at z≃0.05: implications for Ω_{DLA} evolution.
o	Table 1: <[C2001d] QSO JHHMM+DDMM abs N.NNNN> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2002]
[C2002]	(Carraro, 2002)
Write:	<<[C2002] NGC 7036 NNN>> <<[C2002] NGC 7772 NNN>>
N:	331+137
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	CCD UBVI observations in the field of two possible OCR (Open Cluster Remnant) NGC 7036 and NGC 7772.
Ref:	=2002A&A...385..471C
by	CARRARO G.
	Astron. Astrophys., 385, 471-478 (2002)
	Photometry of dissolving star cluster candidates. The cases of NGC 7036 and NGC 7772.
o	Table 2: PG 02331 = PG 0231+051
o	Table ngc7036.dat: <[C2002] NGC 7036 NNN> (Nos 1-331). Table ngc7772.dat: <[C2002] NGC 7772 NNN> (Nos 1-137).
=E=	Catalogue in electronic form as J/A+A/385/471
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2005]
[C2005]	(Colafrancesco, 2005)= ([C2005a]) (Not yet in Simbad)
Write:	<<[C2005] Cavity A>>
N:	2
Object:	Cavity (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Giant X-ray cavitie in 1E 0735.6+7421.
in source:	1E 0735.0+7421
Ref:	=2005A&A...435L...9C
by	COLAFRANCESCO S.
	Astron. Astrophys., 435, 9-12 (2005)
	The SZ effect from cluster cavities.
o	Fig.1: <[C2005] Cavity A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2005a]
[C2005a]	(Colafrancesco, 2005) (Not yet in Simbad)
*****	Avoid the usage of [C2005a], prefer [C2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2006]
[C2006]	(Conselice, 2006)
Write:	<<[C2006] N>>
N:	7
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	LRIS Keck I spectroscopic study of globular clusters associated with the Virgo cluster VCC 1386. Candidate selected from HST WFPC2 images: Among the 7 objects, Nos 5 and 7 are foreground stars, the others are confirmed as globular clusters.
in source:	VCC 1386
Ref:	=2006ApJ...639..120C
by	CONSELICE C.J.
	Astrophys. J., 639, 120-125 (2006)
	Keck spectroscopy of globular clusters in the Virgo cluster dwarf elliptical galaxy VCC 1386.
o	Table 1, Fig.1: <[C2006] N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2007]
[C2007]	(Cheung, 2007)
Write:	<<[C2007] NNN>> <<[C2007] XNN>> <<[C2007] JHHMM+DDMM>>
N:	19+100+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA FIRST images of 'winged' and X-shaped radio source candidates.
Ref:	=2007AJ....133.2097C
by	CHEUNG C.C.
	Astron. J., 133, 2097-2121 (2007)
	FIRST ``Winged'' and X-shaped radio source candidates.
o	Tables 1-2: <[C2007] JHHMM+DDMM> N=100. Table 1: <[C2007] XNN> (Nos X1-X19). Table 2: <[C2007] NNN> (Nos 1-100).
Ref:	=2009ApJS..181..548C
by	CHEUNG C.C. , HEALEY S.E., LANDT H., VERDOES KLEIJN G.A., JORDAN A.
	Astrophys. J., Suppl. Ser., 181, 548-556 (2009)
	FIRST "Winged" and X-shaped radio source candidates. II. New redshifts.
o	Text, Tables 1-2: <[C2007] J1018+2914>.
=E=	Catalogue in electronic form as J/AJ/133/2097
=E=	Catalogue in electronic form as J/ApJS/181/548
Origin	of the Acronym: S = Created by Simbad, the CDS Database
History	of this Acronym: replaces [CHL2009] (for format JHHMM+DDMM)
Details on Acronym: [C2009]
[C2009]	(Campana, 2009)= ([C2009a])
Write:	<<[C2009] SAXJHHMM-N>>
N:	3+2+6+4
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Swift observations of BeppoSAX source fields.
Ref:	=2009ApJ...699.1144C
by	CAMPANA S.
	Astrophys. J., 699, 1144-1152 (2009)
	Linking burst-only X-ray binary sources to faint X-ray transients.
o	Tables 3, 6, 7, 9: <[C2009] SAXJHHMM-N> N=3+2+6+4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2009a]
[C2009a]	(Campana, 2009) (Not yet in Simbad)
*****	Avoid the usage of [C2009a], prefer [C2009]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2009b]
[C2009b]	(Choi, 2009)
Write:	<<[C2009b] N>>
N:	3
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 43.4GHz observations of the Serpens SMM 1 region.
in source:	NAME Serpens Cloud
Ref:	=2009ApJ...705.1730C
by	CHOI M.
	Astrophys. J., 705, 1730-1734 (2009)
	Multiplicity of the protostar Serpens SMM 1 revealed by millimeter imaging.
o	Table 1: <[C2009b] N> (Nos 1-3), <NAME Serpens SMM 1a> (Nos 1a-1b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2009c]
[C2009c]	(Cheung, 2009)
Write:	<<[C2009c] source N>>
N:	5
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Swift XRT observations of N=5 X-ray sources in the field of [YTM2009] J1057-6027.
Ref:	=2009ATel.2083....1C
by	CHEUNG C.C.
	ATel, 2083, 1-1 (2009)
	Swift/XRT Follow-up of the Fermi-LAT Galactic Plane Transient J1057-6027.
o	<[C2009c] source N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2010]
[C2010]	(Caballero, 2010)
Write:	<<[C2010] NN>>
N:	42
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Stars in σ Orionis Cluster. Use of Virtual Observatory tools and data archives.
in source:	NAME sig Ori Cluster
Ref:	=2010A&A...514A..18C
by	CABALLERO J.A.
	Astron. Astrophys., 514A, 18-18 (2010)
	Stars and brown dwarfs in the σ Orionis cluster. II. A proper motion study.
o	Tables A.1-A.2: <[C2010] NN> (Nos 1-42).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2011]
[C2011]	(Comeron, 2011)
Write:	<<[C2011] JHHMMSS.ss+DDMMSS.s>>
N:	17
Object:	(NIR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 and HAWK-I observations of N=17 cool objects in Lupus 3.
in source:	Lupus 3
Ref:	=2011A&A...531A..33C
by	COMERON F.
	Astron. Astrophys., 531A, 33-33 (2011)
	No substellar objects at the center of the Lupus 3 star-forming cloud.
o	Table 3: <[C2011] JHHMMSS.ss+DDMMSS.s> N=17.
o	Table 4 2MASS J16085427-3906575 is a misprint for 2MASS J16085427-3906057.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2011b]
[C2011b]	(Carraro, 2011)
Write:	<<[C2011b] NNNN>>
N:	3003 (SIMBAD class: Star)
Note:	Las Campanas Observatory Swope 1.0m telescope observations of the inner Galactic disk.
Ref:	=2011A&A...536A.101C
by	CARRARO G.
	Astron. Astrophys., 536A, 101-101 (2011)
	Photometric distances to young stars in the inner Galactic disk. I. The L = 314° direction.
o	Table 2 : <[C2011b] NNNN> (Nos 1-3003) N=3003
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2012]
[C2012]	(Comeron, 2012)
Write:	<<[C2012] ESO-HA NNN comp>>
N:	2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT NACO observations of N=2 faint objects at a very small angular distance from the low-mass star ESO-Hα 558 and the possible massive brown dwarf ESO-Hα 566.
in source:	NAME Cha I
Ref:	=2012A&A...537A..97C
by	COMERON F.
	Astron. Astrophys., 537A, 97-97 (2012)
	Discarded candidate companions to low-mass members of Chamaeleon I.
o	Fig. 1, Table 2: <[C2012] ESO-HA NNN comp> (Nos 558 comp, 566 comp).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2019]
[C2019]	(Cloutier, 2019)
Write:	<<[C2019] OI NNNNNNNNN.NN>>
N:	24
Object:	Poss. Pl (SIMBAD class: Planet_Candidate = Extra-solar Planet Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=24 objects of interest ({OI} in format) around 22 stars selected from the TESS Input Catalog (version 7). Use of Gaia DR2 data.
Ref:	=2019AJ....158...81C
by	CLOUTIER R.
	Astron. J., 158, 81-81 (2019)
	The independent discovery of planet candidates around low-mass stars and astrophysical false positives from the first two TESS sectors.
o	Table 5: <[C2019] OI NNNNNNNNN.NN> N=24.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C2021]
[C2021]	(Campana, 2021)
Write:	<<[C2021] CBSNNNNN N>>
N:	18
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Swift XRT observations of N=18 X-ray sources in the Galactic bulge center.
in source:	NAME Galactic Bulge
Ref:	=2021ATel14438....1C
by	CAMPANA S.
	ATel, 4438, 1 (2021)
	Start of the Swift monitoring of the Galactic bulge central part.
o	<[C2021] CBSNNNNN N> N=18.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 4C2
4C2	(4th Cambridge catalog)
*****	Avoid the usage of 4C2, prefer 4C
Details on Acronym: 3C
3C	(3rd Cambridge catalog)
Write:	<<3C NNN>> <<3C NNN.N>> (not recognised by Simbad, but found in literature) <<3C NNNA>> <<3C NNN.NA>>
N:	471
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	The format 'NNN' is sometimes found in the literature as 'NNN.0'. See also 3CR.
Ref:	=1959MmRAS..68...37E
by	EDGE D.O. , SHAKESHAFT J.R., McADAM W.B., BALDWIN J.E., ARCHER S.
	Mem. R. Astron. Soc., 68, 37-60 (1959)
	A survey of radio sources at a frequency of 159 Mc/s.
o	<3C NNN> (Nos 1-471)
=E=	Catalogue in electronic form as VIII/1
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 3C
3C	(3rd Cambridge catalog)
*****	Avoid the usage of 3C, prefer [DP83]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 3C
3C	(3rd Cambridge catalog)
*****	Avoid the usage of 3C, prefer [PUC81]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 3C
3C	(3rd Cambridge catalog)
*****	Avoid the usage of 3C, prefer [UCP83]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 4C
4C	(4th Cambridge catalog)= (4C1) = (4C2)
Write:	<<4C +DD.NN>> <<4C +DD.NN.N>> <<4C +DD.NNA>> (not recognised by Simbad, but found in literature)
N:	4844
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	See also 4CT.
Ref:	=1965MmRAS..69..183P
by	PILKINGTON J.D.H. , SCOTT P.F.
	Mem. R. Astron. Soc., 69, 183-224 (1965)
	A survey of radio sources between declinations 20 and 40.
o	4C +25.56.1 is a 4C source in the declination range +25° lying between 4C +25.56 and 4C +25.57 in right ascension.
o	<4C +DD.NN> N=1218, <4C +DD.NN.N> N=1.
Ref:	=1967MmRAS..71...49G
by	GOWER J.F.R. , SCOTT P.F., WILLS D.
	Mem. R. Astron. Soc., 71, 49-144 (1967)
	A survey of radio sources in the declination ranges -07 to 20 and 40 to 80.
o	<4C +DD.NN> N=3624.
=E=	Catalogue in electronic form as VIII/4
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 5C
5C	(5th Cambridge catalog, part 1)
Write:	<<5C 1.NNNa>>
N:	110
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ν = 408 and 1407 MHz
Ref:	=1966MNRAS.134..189K
by	KENDERDINE S. , RYLE M., POOLEY G.G.
	Mon. Not. R. Astron. Soc., 134, 189-210 (1966)
	Some observations of weak radio sources with the Cambridge one-mile telescope.
o	Table I: <5C 1.NNNa> (Nos 1.1 to 1.106) N=110
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 5C
5C	(5th Cambridge catalog, part 2)
Write:	<<5C 2.NNNa>>
N:	207
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	HPBW = 80"(α ) x100"(δ ) and 23" x30" at 1407MHz.
Ref:	=1968MNRAS.139..529P
by	POOLEY G.G. , KENDERDINE S.
	Mon. Not. R. Astron. Soc., 139, 529-550 (1968)
	The 5C2 Survey of radio-sources.
o	Table I: <5C 2.NNNa> (Nos 2.1 to 2.207) N=211
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 5C
5C	(5th Cambridge catalog, part 3)
Write:	<<5C 3.NNN>>
N:	213
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ν = 408MHz, HPBW = 80" x120". ν = 1407MHz, HPBW = 23" x35".
Ref:	=1969MNRAS.144..101P
by	POOLEY G.G.
	Mon. Not. R. Astron. Soc., 144, 101-127 (1969)
	5C3 : a radio continuum survey of M 31 and its neighbourhood.
o	Table I: <5C 3.NNN> (Nos 3.1 to 3.213)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 5C
5C	(5th Cambridge catalog, part 4)
Write:	<<5C 4.NNN>>
N:	189
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ν = 408MHz, HPBW = 80" x170" ν = 1407MHz, HPBW = 23" x49"
Ref:	=1970MNRAS.151....1W
by	WILLSON M.A.G.
	Mon. Not. R. Astron. Soc., 151, 1-44 (1970)
	Radio observations of the cluster of galaxies in Coma Berenices - The 5C4 survey.
o	Table II: <5C 4.NNN> (Nos 4.1 to 4.189)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 5C
5C	(5th Cambridge catalog, part 5)
Write:	<<5C 5.NNNa>>
N:	250
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1975MNRAS.171..475P
by	PEARSON T.J.
	Mon. Not. R. Astron. Soc., 171, 475-505 (1975)
	The 5C5 survey of radio sources.
o	Table I: <5C 5.NNNa> (Nos 5.1 to 5.250) N=252.
=E=	Catalogue in electronic form as J/MNRAS/171/475
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 5C
5C	(5th Cambridge catalog, part 6)
Write:	<<5C 6.NNNa>>
N:	297
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1978MNRAS.182..273P
by	PEARSON T.J.
	Mon. Not. R. Astron. Soc., 182, 273-274 (1978)
	The 5C6 and 5C7 surveys of radio sources.
o	Table 2: <5C 6.NNNa> (Nos 6.1 to 6.292) N=297. Table 3: <5C 7.NNNa> (Nos 7.1 to 7.271) N=281.
=E=	Catalogue in electronic form as J/MNRAS/182/273
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 5C
5C	(5th Cambridge catalog, part 7)
Write:	<<5C 7.NNNa>>
N:	281
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1978MNRAS.182..273P
by	PEARSON T.J.
	Mon. Not. R. Astron. Soc., 182, 273-274 (1978)
	The 5C6 and 5C7 surveys of radio sources.
o	Table 2: <5C 6.NNNa> (Nos 6.1 to 6.292) N=297. Table 3: <5C 7.NNNa> (Nos 7.1 to 7.271) N=281.
=E=	Catalogue in electronic form as J/MNRAS/182/273
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 5C
5C	(5th Cambridge catalog, part 8)
Write:	<<5C 8.NNN>>
N:	163
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1984MNRAS.211..433G
by	GREEN D.A.
	Mon. Not. R. Astron. Soc., 211, 433-441 (1984)
	Observations of the western part of the Cygnus Loop at 408 MHz : the 5 C8 survey .
o	Table A1: <5C 8.NNN> (Nos 8.1 to 8.163).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 5C
5C	(5th Cambridge catalog, part 9)
Write:	<<5C 9.NNN>>
N:	214
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	N=214, ν = 408 and 1407MHz, near NGP
Ref:	=1977MNRAS.181..547W
by	WAGGETT P.C.
	Mon. Not. R. Astron. Soc., 181, 547-561 (1977)
	The 5C9 survey of radio sources.
o	Table 1: <5C 9.NNN> (Nos 9.1 to 9.214).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 5C
5C	(5th Cambridge catalog, part 10)
Write:	<<5C 10.NNNa>>
N:	313
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	265 sources detected at 408MHz and 48 at 1407MHz.
Ref:	=1981MNRAS.196..695S
by	SCHUCH N.J.
	Mon. Not. R. Astron. Soc., 196, 695-704 (1981)
	The UMa supercluster -I. The optical field and the 5C10 radio survey.
o	Microfiche: <5C 10.NNNa> (Nos 10.1 to 10.278) n=313.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 5C
5C	(5th Cambridge catalog, part 12)
Write:	<<5C 12.NNNa>>
N:	691
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	1982MNRAS.200..747B: 299 sources detected at 408MHz and 65 detected at 1407MHz. Table 1, p. 749 : Recapitulation of data on the 12 5C surveys from 1966 to 1982. 1991MNRAS.251..253B: Extension of the 5C12 catalogue up to No. 691. Table 2: 5C 12+14+15+16 catalogues. Accurate positions (1950 coordinates) for 5C12 sources.
Ref:	=1982MNRAS.200..747B
by	BENN C.R. , GRUEFF G., VIGOTTI M., WALL J.V.
	Mon. Not. R. Astron. Soc., 200, 747-766 (1982)
	A deep radio/optical survey near the North Galactic Pole. I. The 5C12 catalogue.
o	Table 3: <5C12 NNNa> (Nos 12.1-12.316) N=321
Ref:	=1991MNRAS.251..253B
by	BENN C.R. , KENDERDINE S.
	Mon. Not. R. Astron. Soc., 251, 253-266 (1991)
	The 5C14, 5C15, and 5C16 Radio Source Surveys of the 5C12 Area.
o	Table 2: <5C12 NNN> (Nos 12.317-12.691) added
=E=	Catalogue in electronic form as J/MNRAS/200/747
=E=	Catalogue in electronic form as VIII/30
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 5C
5C	(5th Cambridge catalog, part 13)
Write:	<<5C 13.NNNa>>
N:	244
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Ref:	=1995MNRAS.272..699B
by	BENN C.R.
	Mon. Not. R. Astron. Soc., 272, 699-704 (1995)
	The 5C 13 deep radio survey (16h, +42).
o	<5C 13 NNNa> N=244
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 5C
5C	(5th Cambridge catalog, part 20)
Write:	<<5C 20.NNN>>
N:	222
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Survey of N=222 '5C 20.' radio-sources (1.4mJy < S < 12.9mJy) at 408 and 1407MHz. Suggested optical identif. of the sources.
Ref:	=1986MNRAS.222..731B
by	BIRKINSHAW M.
	Mon. Not. R. Astron. Soc., 222, 731-751 (1986)
	A deep survey of Abell 2218 at 408 and 1407 MHz; 5C 20.
o	Table 2: <5C 20.NNN> (Nos 20.1 to 20.222).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [C51]
[C51]	(Courtes, 1951)= (Co) = (Cou)
Write:	<<[C51] NNN>> <<[C51] NNNbis>> <<[C51] NNNA>>
N:	149
Object:	HII (SIMBAD class: HIIReg = HII Region)
Ref:	=1951CR....232..795C
by	COURTES G.
	C.R. Acad. Sci., 232, 795-797 (1951)
	Etude de la Voie Lactee en lumiere monochromatique H-α de 320 a 350° et de 25 a 80° de longitude galactique.
o	<[C51] NNN> (Nos 1-104), <[C51] NNNbis> (Nos 70bis, 92bis) added.
Ref:	=1951CR....232.1283C
by	COURTES G.
	C.R. Acad. Sci., 232, 1283-1285 (1951)
	Etude de la Voie Lactee en lumiere monochromatique H-α de 80 a 180° de longitude galactique.
o	<[C51] NNN> (Nos 105-149), <[C51] NNNA> (Nos 114A-114B) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 6C
6C	(6th Cambridge catalog)
Write:	<<6C HHMM+DDMM>> <<6C HHMMSS+DDMMSS>>
N:	1761+22448
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	The 6th Cambridge Survey of radio-sources covers most of the sky north of Dec = 30' with an angular resolution of 4.2 x4.2 cosec Dec arcmin(2) and a limiting flux density of 120 mJy at 151MHz.
Ref:	=1985MNRAS.217..717B
by	BALDWIN J.E. , BOYSEN R.C., HALES S.E.G., JENNINGS J.E., WAGGETT P.C., WARNER P.J., WILSON D.M.A.
	Mon. Not. R. Astron. Soc., 217, 717-730 (1985)
	The 6C survey of radio sources - I. Declination zone δ > +80.
o	(Erratum) microfiche
o	Table 4: <6C HHMM+DDMM> or <6C HHMMSS+DDMMSS> or <6C BHHMMSS.s+DDMMSS>, N=1761
Ref:	=1988MNRAS.234..919H
by	HALES S.E.G. , BALDWIN J.E., WARNER P.J.
	Mon. Not. R. Astron. Soc., 234, 919-936 (1988)
	The 6C survey of radio sources - II. The zone 30 <δ<51, 08h30m <α<17h30m.
o	<6C HHMM+DDMM> or <6C HHMMSS+DDMMSS> or <6C BHHMMSS.s+DDMMSS>, N=8278
Ref:	=1990MNRAS.246..256H
by	HALES S.E.G. , MASSON C.R., WARNER P.J., BALDWIN J.E.
	Mon. Not. R. Astron. Soc., 246, 256-262 (1990)
	The 6C survey of radio sources - III. The zone 48<Dec<68, 05h25<RA<18h17.
o	<6C HHMM+DDMM> or <6C HHMMSS+DDMMSS> or <6C BHHMMSS.s+DDMMSS>, N=8749
Ref:	=1991MNRAS.251...46H
by	HALES S.E.G. , MAYER C.J., WARNER P.J., BALDWIN J.E.
	Mon. Not. R. Astron. Soc., 251, 46-53 (1991)
	The 6C survey of radio sources - IV. The zone 67 < δ< 82, 0h < α < 24h.
o	<6C HHMM+DDMM> or <6C HHMMSS+DDMMSS> or <6C BHHMMSS.s+DDMMSS>, N=5421
Ref:	=1993MNRAS.262.1057H
by	HALES S.E.G. , MASSON C.R., WARNER P.J., BALDWIN J.E., GREEN D.A.
	Mon. Not. R. Astron. Soc., 262, 1057-1061 (1993)
	The 6C survey of radio sources - V. The zones 6C-Va (48<δ<68, 01h34m<α<06h14m) and 6C-VB (48<δ<68, 17h16m<α<20h24m).
o	<6C HHMM+DDMM> or <6C HHMMSS+DDMMSS> or <6C BHHMMSS.s+DDMMSS>, N=3458
Ref:	=1993MNRAS.263...25H
by	HALES S.E.G. , BALDWIN J.E., WARNER P.J.
	Mon. Not. R. Astron. Soc., 263, 25-30 (1993)
	The 6C survey of radio sources. VI. The continuous zone30<δ<51, Oh<α<09h05m and 22h<α<24h.
o	<6C HHMM+DDMM> or <6C HHMMSS+DDMMSS> or <6C BHHMMSS.s+DDMMSS>, N=6752
=E=	Catalogue in electronic form as VIII/18
=E=	Catalogue in electronic form as VIII/21
=E=	Catalogue in electronic form as VIII/22
=E=	Catalogue in electronic form as VIII/23
=E=	Catalogue in electronic form as VIII/24
=E=	Catalogue in electronic form as VIII/25
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 7C
7C	(7th Cambridge catalog)
Write:	<<7C HHMMSS.ss+DDMMSS.ss>> <<7C HHMM+DDMMa>> <<7C HHMMSS.s+DDMMSS>> <<7C 083231.6+262635A>>
N:	6262+5526+43683
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	7C survey, with the Cambridge Low-Frequency Synthesis Telescope at 151MHz, angular resolution of 70x70 cosec Dec arcsec(2), limiting flux density of 80mJy.
Ref:	=1990MNRAS.246..110M
by	McGILCHRIST M.M. , BALDWIN J.E., RILEY J.M., TITTERINGTON D.J., WALDRAM E.M., WARNER P.J.
	Mon. Not. R. Astron. Soc., 246, 110-122 (1990)
	The 7C survey of radio sources at 151 MHz - two regions centred at RA 10h 28, Dec. 41 and RA 06h 28, Dec. 45.
o	<7C HHMM+DDMMa> N=4723
Ref:	=1995MNRAS.276..614L
by	LACY M. , RILEY J.M., WALDRAM E.M., McMAHON R.G., WARNER P.J.
	Mon. Not. R. Astron. Soc., 276, 614-626 (1995)
	A radio-optical survey of the North Ecliptic Cap.
o	Table 2: <7C HHMM+DDMMa> N=400
Ref:	=1995A&AS..110..419V
by	VISSER A.E. , RILEY J.M., ROETTGERING H.J.A., WALDRAM E.M.
	Astron. Astrophys., Suppl. Ser., 110, 419-439 (1995)
	The 7C survey of radio sources at 151 MHz - a 418-square-° region centred at RA 17h, Dec. 65°.
o	<7C HHMM+DDMMa> N=2702
Ref:	=1996MNRAS.282..779W
by	WALDRAM E.M. , YATES J.A., RILEY J.M., WARNER P.J.
	Mon. Not. R. Astron. Soc., 282, 779-787 (1996)
	The 7C survey of radio sources at 151 MHz - a region covering RA 9h to 16h and Dec. 20 to 35 °.
o	(Erratum) erratum 284, 1007
o	Table A1: <7C HHMMSS.s+DDMMSS> N=5526.
Ref:	=1998MNRAS.294..607V
by	VESSEY S.J. , GREEN D.A.
	Mon. Not. R. Astron. Soc., 294, 607-614 (1998)
	The 7C(G) survey of radio sources at 151 MHz - the Galactic plane at 80° <l< 104° and 126° <l< 180°, for \|b\| <5°.5.
o	Catalogue: <7C(G) HHMM+DDMMa> use <7C HHMM+DDMMa> N=6262.
Ref:	=2007MNRAS.382.1639H
by	HALES S.E.G. , RILEY J.M., WALDRAM E.M., WARNER P.J., BALDWIN J.E.
	Mon. Not. R. Astron. Soc., 382, 1639-1642 (2007)
	A final non-redundant catalogue for the 7C 151-MHz survey.
o	Catalogue: <7C HHMMSS.s+DDMMSS> N=43683.
=E=	Catalogue in electronic form as J/MNRAS/246/110
=E=	Catalogue in electronic form as J/MNRAS/276/614
=E=	Catalogue in electronic form as J/MNRAS/282/779
=E=	Catalogue in electronic form as J/MNRAS/294/607
=E=	Catalogue in electronic form as J/A+AS/110/419
=E=	Catalogue in electronic form as VIII/84
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [C72]
[C72]	(Caswell, 1972)
Write:	<<[C72] GLLL.l+B.b>>
N:	16
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Ref:	=1972AuJPh..25..443C
by	CASWELL J.L.
	Australian J. Phys., 25, 443-450 (1972)
	Hydrogen recombination line and continuum observations at 5000 MHz of 13 southern HII regions.
o	Tables 1, 2: <[C72] GLLL.l+B.b> N=16.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C73]
[C73]	(Cousins, 1973) (Not yet in Simbad)
Write:	<<[C73] FN A>>
N:	13+12+12
Object:	* (SIMBAD class: Star)
in source:	NAME F1 Region
in source:	NAME F2 Region
in source:	NAME F3 Region
Ref:	=1973MmRAS..77..223C
by	COUSINS A.W.J.
	Mem. R. Astron. Soc., 77, 223-None (1973)
	Revised zero points and UBV photometry in the Harvard E and F regions.
o	Data previously published in 1972MNSSA..31..127C.
o	<NAME FN REGION> (Nos F1-F3). Table IV: <[C73] F1 A> (Nos A-N, J missing), <[C73] F2 A> (Nos A-M, J missing), <[C73] F3 A> (Nos A-N, B, J missing).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C74]
[C74]	(Claria, 1974)= (Cl)
Write:	<<[C74] NNN>>
N:	247
Object:	* (SIMBAD class: Star)
Note:	N=247 stars in a field of CMa.
Ref:	=1974AJ.....79.1022C
by	CLARIA J.J.
	Astron. J., 79, 1022-1039 (1974)
	Investigation of a Milky Way region in Canis Majoris.
o	Table V: <[C74] NNN> (Nos 1-247).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C75]
[C75]	(Cohen, 1975)= ([C75a])
Write:	<<[C75] JN>>
N:	6
Object:	Feature (SIMBAD class: Cloud)
Note:	N=6 new HI emission features in the Galactic Center region. See also VDK, [SWP72].
in source:	NAME Gal Center
Ref:	=1975MNRAS.171..659C
by	COHEN R.J.
	Mon. Not. R. Astron. Soc., 171, 659-696 (1975)
	Neutral hydrogen in the Galactic Centre region-I. The Observations.
o	Features 'R' = VDK R, Feature 'E' = [SWP72] E
o	<VDK Ra> (Nos IIIa-IIIb) added. <[C75] JN> (Nos J1-J6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C75a]
[C75a]	(Cohen, 1975)
*****	Avoid the usage of [C75a], prefer [C75]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C75b]
[C75b]	(Cohen, 1975)
Write:	<<[C75b] NN>>
N:	44
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	N=44 IR identified with RAFGL stars.
Ref:	=1975AJ.....80..125C
by	COHEN M.
	Astron. J., 80, 125-127 (1975)
	Optical identifications of AFCRL rocket infrared sources.
o	Table 1: <[C75b] NN> (Nos 1-44).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C77]
[C77]	(Cohen, 1977)
Write:	<<[C77] NN>>
N:	3
Object:	Nebula (SIMBAD class: ISM = Interstellar Medium Object)
Note:	N=3 nebulosity components of CRL 2789.
in source:	RAFGL 2789
Ref:	=1977ApJ...215..533C
by	COHEN M.
	Astrophys. J., 215, 533-540 (1977)
	The nature of V645 Cygni =CRL 2789.
o	Fig.1: <[C77] AN> (Nos N0, N1, N2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 8C
8C	(8th Cambridge catalog)
Write:	<<8C HHMM+DDdA>>
N:	about 5000
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	In the catalogue, 8C objects have no format, and only 1950 coordinates 'HHMMSS+DDMMSS' SIMBAD use the format 'HHMM+DDdA' as found in the references 1992MNRAS.256..404L and 1993MNRAS.263..707L.
Ref:	=1990MNRAS.244..233R
by	REES N.
	Mon. Not. R. Astron. Soc., 244, 233-246 (1990)
	A deep 38-MHz radio survey of the area δ >+60.
o	microfiche MN 244/1-5
o	<8C HHMM+DDdA>
=E=	Catalogue in electronic form as VIII/31
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [C80]
[C80]	(Carter, 1980)= ([C80a])
Write:	<<[C80] NNNN>>
N:	1552
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Table 1: on microfiche 190/1
in source:	SC 0005-34.0
Ref:	=1980MNRAS.190..307C
by	CARTER D.
	Mon. Not. R. Astron. Soc., 190, 307-320 (1980)
	Photometry of the rich cluster of galaxies 0004.8-3450.
o	0004.8-3450 = SC 0005-34.5
o	Microfiche 190/1: <[C80] NNNN> (Nos 1-1552)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C80a]
[C80a]	(Carter, 1980)
*****	Avoid the usage of [C80a], prefer [C80]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C80b]
[C80b]	(Colley, 1980) (Not yet in Simbad)
Write:	<<[C80b] Star NN>>
N:	19
Object:	* (SIMBAD class: Star)
Note:	N=19 stars in the field of DR 15.
Ref:	=1980MNRAS.192..377C
by	COLLEY D.
	Mon. Not. R. Astron. Soc., 192, 377-388 (1980)
	Radio observations of DR 15 at 408, 1407 and 2695 MHz.
o	Figs 1, 2, Table 3: <[I77] DR 15 A> (Nos G-I) added. Fig. 2: <[C80b] Star NN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C81]
[C81]	(Chini, 1981)= (Chini)
Write:	<<[C81] NN>>
N:	38
Object:	* (SIMBAD class: Star)
in source:	NAME rho Oph Cloud
Ref:	=1981A&A....99..346C
by	CHINI R.
	Astron. Astrophys., 99, 346-350 (1981)
	Multicolor photometry of stars in the Ophiuchus dark cloud region.
o	<[C81] NN> N=38
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C83]
[C83]	(Caldwell, 1983)= (DW)
Write:	<<[C83] M 87 DWNN>> <<[C83] NGC NNNN DWNN>> <<[C83] Field DWN>>
N:	27
Object:	dw. Ell. G (SIMBAD class: Galaxy)
Note:	Search for dwarf galaxies in 5 groups of galaxies and a 'general field'.
in source:	NAME M 87 Cluster
in source:	NAME NGC 4472 GROUP
in source:	NAME NGC 4594 GROUP
in source:	NAME NGC 3115 GROUP
in source:	NAME NGC 5846 GROUP
Ref:	=1983AJ.....88..804C
by	CALDWELL N.
	Astron. J., 88, 804-812 (1983)
	Structure and stellar content of dwarf elliptical galaxies.
o	Table I: objets CH 1 to 6 = [S72] 1 to 6
o	Table I: <[C83] M 87 DWNN> (Nos DW1 to DW12), <[C83] NGC 4472 DWNN> N=9 among 10, <[C83] NGC 4594 DWN> (No. DW1), <[C83] NGC 3115 DWN> (No. DW1), <[C83] NGC 5846 DWN> N=3 among 5, <[C83] Field DWN> (No. DW1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: C84
C84	(Crampton+, 1984)= ([C84a]) = (CRX) = (VS)
Write:	<<C84 NNN>>
N:	117
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Einstein Observatory X-ray position for 117 sources around M31, examined with 1000Å.mm⁽-1) slitless spectral plates obtained at the prime focus of the CFHT. Later discussed by Trinchieri and Fabbiano, (TF) Table 1 : (Nos 1-116) a few finding charts
in source:	M 31 = NGC 224
Ref:	=1984ApJ...284..663C
by	CRAMPTON D. , COWLEY A.P., HUTCHINGS J.B., SCHADE D.J., VAN SPEYBROECK L.P.
	Astrophys. J., 284, 663-669 (1984)
	Optical counterparts for X-ray sources in M 31.
o	Table 1: <C84 NNN> N=116
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [C84a]
[C84a]	(Crampton+, 1984)
*****	Avoid the usage of [C84a], prefer C84
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C84b]
[C84b]	(Chen, 1984)
Write:	<<[C84b] HHMM+DDdA>>
N:	137
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Note:	Figs.1: Finding Charts
Ref:	=1984A&A...134..306C
by	CHEN J.-S.
	Astron. Astrophys., 134, 306-318 (1984)
	A study of optically selected QSOs in a field centered at 01h39m,-55d.
o	Table 2: <[C84b] HHMM-DDdA> N=137
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C84c]
[C84c]	(Campbell, 1984)= (RC)
Write:	<<[C84c] N>> <<[C84c] IR>> <<[C84c] H2O>>
N:	5+1+1
Object:	(Rad) + (IR) + Maser (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=5 radio + N=1 IR + N=1 H2O maser in AFGL 2591.
in source:	RAFGL 2591
Ref:	=1984ApJ...287..334C
by	CAMPBELL B.
	Astrophys. J., 287, 334-337 (1984)
	New radio sources at AFGL 2591 : young cluster or single star ?
o	Table 1: <[C84c] N> (Nos 1-4), <[C84c] IR> N=1, <[C84c] H2O> N=1.
Ref:	=1992ApJ...391..710T
by	TAMURA M. , YAMASHITA T.
	Astrophys. J., 391, 710-718 (1992)
	Infrared morphology of mass outflow from GL 2591.
o	Fig.1a, Table 3: <[TGJ91] AFGL 2591 NIRS N> (Nos 6-8) added. Fig.1c, Table 2: <[TY92] A> (Nos A-D). Fig.4d: <[C84c] N> (No. 5) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C86]
[C86]	(Clark, 1986)
Write:	<<[C86] L988 a>>
N:	6
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Radio observations of [C86] L988 a, c, e, f, which are stars with molecular flows.
in source:	LDN 988
Ref:	=1986A&A...164L..19C
by	CLARK F.O.
	Astron. Astrophys., 164, 19-21 (1986)
	The pincushion cloud : the bipolar flows in L 988.
o	Table 1: <[C86] L988 a> (Nos a-f)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C87]
[C87]	(Cristiani, 1987)= (C) = ([C87a])
Write:	<<[C87] NN>>
N:	51
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=51 stars in the field of QSO 1209+107
Ref:	=1987A&A...175L...1C
by	CRISTIANI S.
	Astron. Astrophys., 175, 1-4 (1987)
	Observation of the HII galaxy giving origin to the z = 0.3930 absorption system of the QSO 1209+107.
o	Table 1: <[C87] NN> (Nos 1-51)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C87a]
[C87a]	(Cristiani, 1987)
*****	Avoid the usage of [C87a], prefer [C87]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C87b]
[C87b]	(Cook, 1987)
Write:	<<[C87b] NN>>
N:	26
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Note:	N=26 carbon stars in SagDIG galaxy, from Cook K.H. PhD. Thesis, Univ. Arizona.
in source:	NAME Sag dIG
Ref:	=2002AJ....123..238D
by	DEMERS S. , BATTINELLI P.
	Astron. J., 123, 238-243 (2002)
	C star survey of local group dwarf galaxies. III. The Sagittarius dwarf irregular and the Leo I dwarf spheroidal galaxies.
o	Table 5: Numbering from Cook K.H. PhD. Thesis, Univ. Arizona, 1987.
o	Table 3: <[DB2002] SagDIG CNN> (Nos C01-C16). Table 4: <[DB2002] Leo I CNN> (Nos C01-C13). Table 5: <[C87b] NN> (Nos 1-26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C88]
[C88]	(Cohen, 1988)
Write:	<<[C88] NGC 4406 NNN>> <<[C88] NGC 4472 NNN>>
N:	164+292
Object:	? (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	Table II: point sources in the field of NGC 4406, (Nos 1-164) Table III: point sources in the field of NGC 4472, (Nos 1-292)
in source:	NGC 4406 = M 86
in source:	NGC 4472 = M 49
Ref:	=1988AJ.....95..682C
by	COHEN J.G.
	Astron. J., 95, 682-703 (1988)
	The globular cluster systems of three Virgo ellipticals.
o	Table II: <[C88] NGC 4406 NNN> (Nos 1-164). Table III: <[C88] NGC 4472 NNN> (Nos 1-292).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C89]
[C89]	(Chavira, 1989)= (ChaG)
Write:	<<[C89] NNN>>
N:	121
Object:	G (SIMBAD class: Galaxy)
Note:	Identif. charts No. 64 missing.
Ref:	=1989RMxAA..17..109C
by	CHAVIRA E.
	Rev. Mex. Astron. Astrofis., 17, 109-110 (1989)
	New list of blue galaxies.
o	Table 1: <[C89] NN> (Nos 1-24)
Ref:	=1996RMxAA..32..131C
by	CHAVIRA E.
	Rev. Mex. Astron. Astrofis., 32, 131-134 (1996)
	A list of new blue galaxies. II.
o	Table 1: <[C89] NN> (Nos 25-63)
Ref:	=1998RMxAA..34..105C
by	CHAVIRA E. , LOPEZ A.
	Rev. Mex. Astron. Astrofis., 34, 105-110 (1998)
	A list of new blue galaxies. III.
o	Table 1: <[C89] NNN> (Nos 65-122).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 9C
9C	(9th Cambridge catalog)
Write:	<<9C JHHMM+DDMMa>>
N:	242+643
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	9C survey: Ryle Telescope 15.2GHz observations of N=242+643 sources.
Ref:	=2003MNRAS.342..915W
by	WALDRAM E.M. , POOLEY G.G., GRAINGE K.J.B., JONES M.E., SAUNDERS R.D.E., SCOTT P.F., TAYLOR A.C.
	Mon. Not. R. Astron. Soc., 342, 915-925 (2003)
	9C: a survey of radio sources at 15 GHz with the Ryle Telescope.
o	p.920: Fig.11 and 12, variable sources J0930+350 = 9C J0930+3503, J1521+436 = 9C J1521+4366.
o	Tables 4-6: <9C JHHMM+DDMM> N=84+103+55.
Ref:	=2010MNRAS.404.1005W
by	WALDRAM E.M. , POOLEY G.G., DAVIES M.L., GRAINGE K.J.B., SCOTT P.F.
	Mon. Not. R. Astron. Soc., 404, 1005-1017 (2010)
	9C continued: results from a deeper radio-source survey at 15 GHz.
o	<9C JHHMM+DDMMa> N=643.
=E=	Catalogue in electronic form as <J/MNRAS/342/915/>
=E=	Catalogue in electronic form as <J/MNRAS/404/1005/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [C90]
[C90]	(Cernis, 1990)
Write:	<<[C90] NN>>
N:	78
Object:	* (SIMBAD class: Star)
in source:	NGC 1333
Ref:	=1990Ap&SS.166..315C
by	CERNIS K.
	Astrophys. Space Sci., 166, 315-330 (1990)
	Interstellar extinction in the vicinity of the reflection nebula NGC 1333 in Perseus.
o	Table II: <[C90] NN> (Nos 1-78).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C91]
[C91]	(Casali, 1991)= ([C91a]) = (IRS)
Write:	<<[C91] IRS N>>
N:	2
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	Reipurth 50
Ref:	=1991MNRAS.248..229C
by	CASALI M.M.
	Mon. Not. R. Astron. Soc., 248, 229-232 (1991)
	The Reipurth 50 - north infrared source.
o	<[C91] IRS N> (Nos 1-2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C91a]
[C91a]	(Casali, 1991)
*****	Avoid the usage of [C91a], prefer [C91]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C91b]
[C91b]	(Campusano, 1991)
Write:	<<[C91b] HHMMm-DDMM>>
N:	61
Object:	QSO (SIMBAD class: QSO = Quasar)
Note:	A 2nd ref., 1991AJ....102..502C, gives redshifts of 35 of these objects
Ref:	=1991A&A...250....9C
by	CAMPUSANO L.E.
	Astron. Astrophys., 250, 9-22 (1991)
	Assemblage of two UVX-QSO samples to B 19 in the vicinity of the South Galactic Pole.
o	Table 3: <[C91b] HHMMm+DDMM> N=61
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C92]
[C92]	(Cananzi, 1991)
Write:	<<[C92] OBNN-N>> <<[C92] OBNN-WRN>>
N:	9
Object:	* (SIMBAD class: WolfRayet* = Wolf-Rayet)
Stat:	is completely incorporated in Simbad
Note:	Table 6: Stars in OB associations ('OBNN' in the format), 'OBNN' = '[V64] NN' in SIMBAD. format 'OB33-N': N=1 WR?. format 'OBNN-WRN': WR* in OB 33 (N=3), in OB 32 (N-1), in OB 42 (N=1), in OB 59 (N=1) and in OB 69 (N=2).
in source:	M 31 = NGC 224
Ref:	=1992A&A...259...17C
by	CANANZI K.
	Astron. Astrophys., 259, 17-24 (1992)
	Massive star population in M 31 OB associations.
o	Table 6: <[C92] OBNN-N> N=1, <[C92] OBNN-WRN> N=8
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C93]
[C93]	(Cernis, 1993)= ([C93a])
Write:	<<[C93] NNN>>
N:	189
Object:	* (SIMBAD class: Star)
Note:	Table 1: photometry of stars (Nos 1-189): These stars are in the vicinity of LDN 1470 (Table 2), or in the vicinity of IC 348 (Table 4), or in the region of the assoc. Per OB 2.
Ref:	=1993BaltA...2..214C
by	CERNIS K.
	Baltic Astronomy, 2, 214-240 (1993)
	Interstellar extinction in the direction of the open cluster IC 348 and the Per OB2 association.
o	<[C93] NNN> N=189
=E=	Catalogue in electronic form as II/197
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C93a]
[C93a]	(Cernis, 1993)
*****	Avoid the usage of [C93a], prefer [C93]
Details on Acronym: [C93b]
[C93b]	(Cunow, 1993)
Write:	<<[C93b] ACO NNNN NN>> <<[C93b] ACO S NNNN NN>>
N:	270
Object:	G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 3: format 'ACO S 1172 NN', N=18 Table 4: format 'ACO 2734 NN', N=10 Table 5: format 'ACO 42 NN', N=31 Table 6: format 'ACO 2778 NN', N=17 Table 7: format 'ACO S 83 NN', N=17 Table 8: format 'ACO 140 NN', N=16 Table 9: format 'ACO S 133 NN', N=16 Table 10: format 'ACO 2911 NN', N=18 Table 11: format 'ACO 3054 NN', N=16 Table 12: format 'ACO 3698 NN', N=30 Table 13: format 'ACO 3705 NN', N=47 Table 14: format 'ACO 3775 NN', N=19 Table 15: format 'ACO 3805 NN', N=15
in source:	ACO S 1172
in source:	ACO 2734
in source:	ACO 42
in source:	ACO 2778
in source:	ACO S 83
in source:	ACO 140
in source:	ACO S 133
in source:	ACO 2911
in source:	ACO 3054
in source:	ACO 3698
in source:	ACO 3705
in source:	ACO 3775
in source:	ACO 3805
Ref:	=1993A&AS...97..541C
by	CUNOW B.
	Astron. Astrophys., Suppl. Ser., 97, 541-548 (1993)
	Photometric CCD sequences in 13 southern Abell clusters.
o	Tables 3 to 15: <[C93b] ACO NNNN NN> or <[C93b] ACO S NNNN NN> N=270
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C96]
[C96]	(Corral, 1996)
*****	Avoid the usage of [C96], prefer [S92b]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C97]
[C97]	(Chanturiya, 1997)
Write:	<<[C97] NN>>
N:	74
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1997AN....318..369C
by	CHANTURIYA S.M.
	Astron. Nachr., 318, 369-386 (1997)
	Proper motions, absolute magnitudes and spatial distribution of zirconium stars.
o	Table 5: <[C97] NN> (Nos 1-74)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [C99]
[C99]	(Cohen, 1999)
Write:	<<[C99] M13ms JHHMMSSs+DDMMSS>> <<[C99] M71ms BHHMMSSs+DDMMSS>>
N:	50+78
Object:	main-sequence * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Studies of main-sequence stars ('ms' in the format) in globular clusters. In M13, stars are given with a J2000 format, In M71, stars are given with a B1950 format.
in source:	M 13 = NGC 6205
in source:	M 71 = NGC 6838
Ref:	=1999AJ....117.2428C
by	COHEN J.G.
	Astron. J., 117, 2428-2433 (1999)
	The spectra of main-sequence stars in galactic globular clusters. I. CH and CN bands in M13.
o	T.1: [C99] M13ms J1641942+362438 = [C99] M13ms J1642342+362438 in SIMBAD
o	Table 1: <[C99] M13ms JHHMMSSs+DDMMSS> N=50.
Ref:	=1999AJ....117.2434C
by	COHEN J.G.
	Astron. J., 117, 2434-2439 (1999)
	The spectra of main-sequence stars in galactic globular clusters. II. CH and CN bands in M71.
o	Table 1: <[C99] M71ms BHHMMSSs+DDMMSS> N=78.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CA
CA	(C. Aspin)
*****	Avoid the usage of CA, prefer [A98b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Ca
Ca	(Calan obs.)= (MQCG)
Write:	<<Ca HHMM+DDd>>
N:	6
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Ref:	=1975ApJ...198L..97M
by	MELNICK J. , QUINTANA H.
	Astrophys. J., 198, 97-99 (1975)
	Southern galaxy clusters identified with 3U X-ray sources.
o	<CA HHMM-DDd> N=6
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Ca
Ca	(Calar Alto obs.)
*****	Avoid the usage of Ca, prefer [WEB76]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CA
CA	(CADIS)
*****	Avoid the usage of CA, prefer [WMT98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CA2002]
[CA2002]	(Clemens+Alexander, 2002)
Write:	<<[CA2002] Na>>
N:	8
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	SCUBA and MERLIN images of NGC 4490, Halpha INT data: search for 84GHz sources that coincide with an HII region.
in source:	NGC 4490
Ref:	=2002MNRAS.333...39C
by	CLEMENS M.S. , ALEXANDER P.
	Mon. Not. R. Astron. Soc., 333, 39-46 (2002)
	Hα , SCUBA and MERLIN imaging of NGC 4490.
o	Table 1: <[CA2002] Na> (Nos 1-3, 4a-4b, 5-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: caa
caa	(Caseopeia, field A)
*****	Avoid the usage of caa, prefer [ABC90]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CAA2000]
[CAA2000]	(Cristiani+Appenzeller+Arnouts+, 2000)= (EIS)
Write:	<<[CAA2000] EIS NN>> <<[CAA2000] EIS ANN>> <<[CAA2000] ANON NN>>
N:	11+10+9
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT FORS observations. Tables 2, 3: In the formats 'EIS' stands for ESO Imaging Survey. 'EIS NN' are Lyman-Break candidates in an EIS list, in the HDFS field. 'EIS ANN' are Lyman-Break candidates in an EIS list, in AXAF fields 'U' and 'B'. 'ANON NN' are random-chosen objects.
Ref:	=2000A&A...359..489C
by	CRISTIANI S. , APPENZELLER I., ARNOUTS S., NONINO M., ARAGON-SALAMANCA A., BENOIST C., DA COSTA L., DENNEFELD M., RENGELINK R., RENZINI A., SZEIFERT T., WHITE S.
	Astron. Astrophys., 359, 489-492 (2000)
	The first VLT FORS1 spectra of Lyman-break candidates in the HDF-S and AXAF Deep Field.
o	Tables 2, 3: <[CAA2000] EIS NN> N=11 among (Nos 18-60), <[CAA2000] EIS ANN> N=10 among (Nos U01-U28 and B02-B12), <[CAA2000] ANON NN> N=9 among (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CAA2003]
[CAA2003]	(Castro-Rodriguez+Aguerri+Arnoboldi+, 2003)
Write:	<<[CAA2003] JHHMMSS.sss+DDMMSS.ss>> <<[CAA2003] IGNA>>
N:	29+4
Object:	Poss. PN (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
Stat:	is completely incorporated in Simbad
Note:	La Silla 2.2m telescope and FORS2 VLT observations. N=29 PN candidates in the Leo group + 2 emission-line candidates, IG 2 with 2 emission components.
in source:	NAME LEO GROUP = NAME M 96 GROUP
Ref:	=2003A&A...405..803C
by	CASTRO-RODRIGUEZ N. , AGUERRI J.A.L., ARNABOLDI M., GERHARD O., FREEMAN K.C., NAPOLITANO N.R., CAPACCIOLI M.
	Astron. Astrophys., 405, 803-812 (2003)
	Narrow band survey for intragroup light in the Leo HI cloud. Constraints on the galaxy background contamination in imaging surveys for intracluster planetary nebulae.
o	Table 2: <[CAA2003] JHHMMSS.sss+DDMMSS.ss> N=29. Table 4: <[CAA2003] IGNA> (Nos IG1, IG2, IG2A, IG2B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CAA2009]
[CAA2009]	(Castro-Rodriguez+Arnaboldi+Aguerri+, 2009)
Write:	<<[CAA2009] RCNN-NN>> <<[CAA2009] LPRX-N>> <<[CAA2009] LPS-N>> <<[CAA2009] LPE-NN>> <<[CAA2009] LSF-NN>> <<[CAA2009] SUBN-NN>>
N:	28+9+7+20+23+13+11
Object:	Em. Obj. (SIMBAD class: EmObj = Emission Object)
Note:	INT WFC, ESO/MPI WFI and Subaru Suprime-Cam broad- and narrow-band observations of emission-line objects in the Virgo Cluster.
in source:	NAME Virgo Cluster
Ref:	=2009A&A...507..621C
by	CASTRO-RODRIGUEZ N. , ARNABOLDI M., AGUERRI J.A.L., GERHARD O., OKAMURA S., YASUDA N., FREEMAN K.C.
	Astron. Astrophys., 507, 621-634 (2009)
	Intracluster light in the Virgo cluster: large scale distribution.
o	Table A.1: <[CAA2009] RCN1-NN> (Nos 1-28). Table A.2: <[CAA2009] LPRX-N> (Nos 1-9). Table A.3: <[CAA2009] LPS-N> (Nos 1-7). Table A.4: <[CAA2009] LPE-NN> (Nos 1-20). Table A.5: <[CAA2009] LPF-NN> (Nos 1-23). Table A.6: <[CAA2009] SUB2-NN> (Nos 1-13). Table A.7: <[CAA2009] SUB3-NN> (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CAA97]
[CAA97]	(Covino+Alcala+Allain+, 1997)
Write:	<<[CAA97] RX JHHMM.m+DDMMW>>
N:	5
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=5 possible optical counterpart of the corresponding RX J See also [AKS95b], [ATW96], [WKS96], [MMS97], [KWS97], [WSK97], [HMC99].
Ref:	=1997A&A...328..187C
by	COVINO E. , ALCALA J.M., ALLAIN S., BOUVIER J., TERRANEGRA L., KRAUTTER J.
	Astron. Astrophys., 328, 187-202 (1997)
	A study of the Chamaeleon star-forming region from the ROSAT all-sky survey. III. High resolution spectroscopic study.
o	p.200 : Cloud FS 195 not identified
o	Table 2: <[CAA97] RX JHHMM.m+DDMMW> N=5
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: cab
cab	(Caseopeia, field B)
*****	Avoid the usage of cab, prefer [ABC90]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CAB2000]
[CAB2000]	(Colina+Arribas+Borne+, 2000)
Write:	<<[CAB2000] Nw>> <<[CAB2000] RN>>
N:	2+2
Object:	Region (SIMBAD class: PartofG = Part of a Galaxy)
Note:	HST and WHT imaging of the galaxy IRAS 12112+0305. N=2 Nuclei, Nuclei north and Nuclei South, 'Nn' and 'Ns'. See also [CGM90]. N=2 other dominant regions, (Nos R1-R2).
in source:	IRAS 12112+0305
Ref:	=2000ApJ...533L...9C
by	COLINA L. , ARRIBAS S., BORNE K.D., MONREAL A.
	Astrophys. J., 533, 9-12 (2000)
	Detection and mapping of decoupled stellar and ionized gas structures in the ultraluminous infrared galaxy IRAS 12112+0305.
o	Table 1: <[CAB2000] Nw> (Nos Nn, Ns), <[CAB2000] RN> (Nos R1-R2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CAB2001]
[CAB2001]	(Cappellaro+Altavilla+Benetti+, 2001)
Write:	<<[CAB2001] JHHMMSS.s+DDMMSS>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=3 host galaxies of SN 2001BC, SN 2001BD, and SN 2001BE. For SN 2001BC see also [DFN2001].
Ref:	=2001IAUC.7615....1C
by	CAPPELLARO E. , ALTAVILLA G., BENETTI S., PASTORELLO A., TURATTO M., CLOCCHIATTI A., DANZIGER I.J., MAZZALI P., PATAT F.
	IAU Circ., 7615, 1-None (2001)
	Supernovae 2001bc, 2001bd, 2001be.
o	<[CAB2001] JHHMMSS.s+DDMMSS> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CAB2004]
[CAB2004]	(Cristiani+Alexander+Bauer+, 2004)
Write:	<<[CAB2004] JHHMMSS.ss+DDMMSS.s>>
N:	11+6
Object:	Poss. QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	GOODS (Great Observatories Origins Deep Survey) search for QSOs with high redshifts. ACS Hubble observations are matched with Chandra ACIS from CXOCDFS and [ABB2003]. N=11 candidates are found in the GOODS South Field (sub-field of CDFS), and N=6 in the GOODS North Field (sub-field of HDFN).
in source:	NAME GOODS North Field
in source:	NAME GOODS South Field
in source:	NAME HDFN
in source:	NAME CDFS
Ref:	=2004ApJ...600L.119C
by	CRISTIANI S. , ALEXANDER D.M., BAUER F., BRANDT W.N., CHATZICHRISTOU E.T., FONTANOT F., GRAZIAN A., KOEKEMOER A., LUCAS R.A., MONACO P., NONINO M., PADOVANI P., STERN D., TOZZI P., TREISTER E., URRY C.M., VANZELLA E.
	Astrophys. J., 600, 119-122 (2004)
	The space density of high-redshift QSOs in the Great Observatories Origins Deep Survey.
o	Table 1: <[CAB2004] JHHMMSS.ss+DDMMSS.s> N=11+6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CAB2008]
[CAB2008]	(Chapin+Ade Bock+, 2008)= (BLAST)
Write:	<<[CAB2008] VNN>>
N:	60
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	Balloon-borne Large Aperture Submillimeter Telescope (BLAST) survey in the Vulpecula region. See also BLAST.
in source:	NAME Vulpecula Region
Ref:	=2008ApJ...681..428C
by	CHAPIN E.L. , ADE P.A.R., BOCK J.J., BRUNT C., DEVLIN M.J., DICKER S., GRIFFIN M., GUNDERSEN J.O., HALPERN M., HARGRAVE P.C., HUGHES D.H., KLEIN J., MARSDEN G., MARTIN P.G., MAUSKOPF P., NETTERFIELD C.B., OLMI L., PASCALE E., PATANCHON G., REX M., SCOTT D., SEMISCH C., TRUCH M.D.P., TUCKER C., TUCKER G.S., VIERO M.P., WIEBE D.V.
	Astrophys. J., 681, 428-452 (2008)
	The balloon-borne large aperture submillimeter telescope (BLAST) 2005: a 4 °^{2} galactic plane survey in Vulpecula (l = 59°).
o	Table 2, col(1): <[CAB2008] VNN> (Nos V01-V60) = Table 2, col(2): <BLAST JHHMMSS+DDMMSS> N=60.
=E=	Catalogue in electronic form as J/ApJ/681/428
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CAB2011]
[CAB2011]	(Culverhouse+Ade+Bock+, 2011)
Write:	<<[CAB2011] GLLL.ll+BB.bb>>
N:	505+4
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	QUaD 2.6m Cassegrain radio telescope observations at 100 and 150GHz of compact sources found in the QUaD Galactic Plane Survey.
Ref:	=2011ApJS..195....8C
by	CULVERHOUSE T. , ADE P., BOCK J., BOWDEN M., BROWN M.L., CAHILL G., CASTRO P.G., CHURCH S., FRIEDMAN R., GANGA K., GEAR W.K., GUPTA S., HINDERKS J., KOVAC J., LANGE A.E., LEITCH E., MELHUISH S.J., MEMARI Y., MURPHY J.A., ORLANDO A., PRYKE C., SCHWARZ R., O'SULLIVAN C., PICCIRILLO L., RAJGURU N., RUSHOLME B., TAYLOR A.N., THOMPSON K.L., TURNER A.H., WU E.Y.S., ZEMCOV M., (The QUaD Collaboration)
	Astrophys. J., Suppl. Ser., 195, 8 (2011)
	The QUaD Galactic Plane Survey. II. A compact source catalog.
o	Tables 2-3: <[CAB2011] GLLL.ll+BB.bb> N=505+4.
=E=	Catalogue in electronic form as <J/ApJS/195/8/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CAB2014]
[CAB2014]	(Chavarria+Allen+Brunt+, 2014)
Write:	<<[CAB2014] W5-east NNN>> <<[CAB2014] S235 NNNN>> <<[CAB2014] S252 NNNN>> <<[CAB2014] S255 NNNN>> <<[CAB2014] NGC7538 NNNN>>
N:	2509
Object:	Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Note:	Flamingos and MMT SWIRC NIR observations of N=2509 YSOs in N=4 massive star-forming regions. Use of Spitzer IRAC archival data. See also [CAH2008].
in source:	NAME W 5 East
in source:	SH 2-235
in source:	SH 2-252
in source:	NGC 7538
Ref:	=2014MNRAS.439.3719C
by	CHAVARRIA L. , ALLEN L., BRUNT C., HORA J.L., MUENCH A., FAZIO G.
	Mon. Not. R. Astron. Soc., 439, 3719-3754 (2014)
	A multiwavelength study of embedded clusters in W5-east, NGC 7538, S235, S252 and S254-S258.
o	Table 2: <[CAB2014] W5-east NNN> (Nos 1-478), <[CAB2014] S235 NNNN> (Nos 479-1168), <[CAB2014] S252 NNNN> (Nos 1169-1847), <[CAB2014] S255 NNNN> (Nos 1848-2359), <[CAB2014] NGC7538 NNNN> (Nos 2360-3021).
=E=	Catalogue in electronic form as <J/MNRAS/439/3719/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CAB95]
[CAB95]	(Condon+Anderson+Broderick, 1995)
Write:	<<[CAB95] IRAS FHHMMm+DDMM>>
N:	354
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	N=354 radio identifications of extragalactic IRAS Faint Source Catalog (version 2).
Ref:	=1995AJ....109.2318C
by	CONDON J.J. , ANDERSON E., BRODERICK J.J.
	Astron. J., 109, 2318-2354 (1995)
	Radio identifications of extragalactic IRAS sources.
o	Table 1 :<[CAB95] IRAS FHHMMm+DDMM> N=354.
=E=	Catalogue in electronic form as J/AJ/109/2318
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CABS
CABS	(Chromospherically Active Binary Stars)
Write:	<<CABS NNN>>
N:	206
Object:	SB (SIMBAD class: SB* = Spectroscopic Binary)
Stat:	is completely incorporated in Simbad
Note:	2nd edition: supersedes CCABS with a different numbering. Superseded by the third edition CABS III with a different numbering.
Ref:	=1993A&AS..100..173S
by	STRASSMEIER K.G. , HALL D.S., FEKEL F.C., SCHECK M.
	Astron. Astrophys., Suppl. Ser., 100, 173-225 (1993)
	A catalog of chromospherically active binary stars (second edition).
o	T.1: <CABS NNN> (Nos 1-206)
=E=	Catalogue in electronic form as V/76
Origin	of the Acronym: L (1996Ap&SS.236..215B)
Details on Acronym: CABS III
CABS III	(Chromospherically Active Binary Stars, 3rd ed.)
Write:	<<CABS III NNN>>
N:	409
Object:	SB (SIMBAD class: SB* = Spectroscopic Binary)
Note:	3rd edition: supersedes CABS with a different numbering.
Ref:	=2008MNRAS.389.1722E
by	EKER Z. , FILIZ AK N., BILIR S., DOGRU D., TUYSUZ M., SOYDUGAN E., BAKIS H., UGRAS B., SOYDUGAN F., ERDEM A., DEMIRCAN O.
	Mon. Not. R. Astron. Soc., 389, 1722-1726 (2008)
	A catalogue of chromospherically active binary stars (third edition).
o	Catalog: <CABS III NNN> (Nos 1-409).
=E=	Catalogue in electronic form as V/128
=E=	Catalogue in electronic form as <J/MNRAS/389/1722/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CAC2009]
[CAC2009]	(Coziol+Andernach+Caretta+, 2009)
Write:	<<[CAC2009] ANNNNA a>> <<[CAC2009] SNNNNA a>> <<[CAC2009] JHHMMSS.s+DDMMSS.s>>
N:	1426+1
Object:	Poss. BCG + G (SIMBAD class: Galaxy)
Note:	N=1426 candidate brightest cluster members (BCM) located in 1169 different Abell clusters. Format JHHMMSS.s+DDMMSS.s: for N=1 rejected candidate without cross-identification.
Ref:	=2009AJ....137.4795C
by	COZIOL R. , ANDERNACH H., CARETTA C.A., ALAMO-MARTINEZ K.A., TAGO E.
	Astron. J., 137, 4795-4809 (2009)
	The dynamical state of brightest cluster galaxies and the formation of clusters.
o	(Erratum) erratum vol. 142, art. 142 (2011)
o	Table 1: <[CAC2009] ANNNNA a> N=1426. Table 2: <[CAC2009] JHHMMSS.s+DDMMSS.s> N=1.
=E=	Catalogue in electronic form as J/AJ/137/4795
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CAC2011]
[CAC2011]	(Carraro+Anthony-Twarog+Costa+, 2011) (Not yet in Simbad)
Write:	<<[CAC2011] DDD.dddd+DD.dddd>>
N:	15444+3661
Object:	* (SIMBAD class: Star)
Note:	CTIO 1m and 0.9m telescope observations of N= 15444+3661 in the field of the open cluster NGC 5822.
in source:	NGC 5822
Ref:	=2011AJ....142..127C
by	CARRARO G. , ANTHONY-TWAROG B.J., COSTA E., JONES B.J., TWAROG B.A.
	Astron. J., 142, 127 (2011)
	A UBVI and uvbyCaHβ analysis of the intermediate-age open cluster, NGC 5822.
o	Tables 3+5: <[CAC2011] DDD.dddd+DD.dddd> N=15444+3661.
=E=	Catalogue in electronic form as J/AJ/142/127
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CAC2014]
[CAC2014]	(Chow-Martinez+Andernach+Caretta+, 2014)
Write:	<<[CAC2014] {A\|S}NNNNA>>
N:	1795+523
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	List of "line-of-sight components" of Abell/ACO clusters. A final uppercase letter in the format is used, in increasing order of redshift, whenever a cluster shows more than one concentration along the line of sight, separated in redshift by more than ∼1500km/s. See also MSCC, SSCC.
Ref:	=2014MNRAS.445.4073C
by	CHOW-MARTINEZ M. , ANDERNACH H., CARETTA C.A., TREJO-ALONSO J.J.
	Mon. Not. R. Astron. Soc., 445, 4073-4085 (2014)
	Two new catalogues of superclusters of Abell/ACO galaxy clusters out to redshift 0.15.
o	Table 1: <MSCC NNN> (Nos 1-601). Table 2: <SSCC NNN> (Nos 1-423). Table 3: <[CAC2014] ANNNNA> N=1795 among (Nos A0008A-A4074A), <[CAC2014] SNNNNA> N=523 among (Nos S0006A-S1172D).
=E=	Catalogue in electronic form as <J/MNRAS/445/4073/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: cad
cad	(Caseopeia, field D)
*****	Avoid the usage of cad, prefer [ABC90]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CAD2006]
[CAD2006]	(COvone+Adami+DUrret+, 2006)
Write:	<<[CAD2006] DSN>> <<[CAD2006] ComDif>>
N:	2+1
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Archival HST WFPC2 images of ACO 2667: N=2 Diffuse Sources (letters DS in the format) and N=1 Compact Diffuse (ComDif) source are found. See also [CKS2006].
in source:	ACO 2667
Ref:	=2006A&A...460..381C
by	COVONE G. , ADAMI C., DURRET F., KNEIB J.-P., LIMA NETO G.B., SLEZAK E.
	Astron. Astrophys., 460, 381-391 (2006)
	Diffuse light and building history of the galaxy cluster Abell 2667.
o	Table 1: <[CAD2006] DSN> (Nos DS1, DS2), <[CAD2006] ComDif> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CAD2012]
[CAD2012]	(Chen+Arce+Dunham+, 2012)
Write:	<<[CAD2012] CB 17 MMS>>
N:	1
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	SMA 1.3mm observations of Bok globule [CB88] 17.
in source:	[CB88] 17
Ref:	=2012ApJ...751...89C
by	CHEN X. , ARCE H.G., DUNHAM M.M., ZHANG Q., BOURKE T.L., LAUNHARDT R., SCHMALZL M., HENNING T.
	Astrophys. J., 751, 89 (2012)
	Submillimeter array and Spitzer observations of Bok globule CB 17: a candidate first hydrostatic core?
o	<[CAD2012] CB 17 MMS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CAD2014]
[CAD2014]	(Coldwell+Alonso+Duplancic+, 2014)
Write:	<<[CAD2014] NN>>
N:	15
Object:	G in ClG (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT 4.1m VISTA VIRCAM telescope observations of N=15 candidate cluster member galaxies of Suzaku J1759-3450. Use of data from the ESO VVV survey.
in source:	Suzaku J1759-3450
Ref:	=2014A&A...569A..49C
by	COLDWELL G. , ALONSO S., DUPLANCIC F., HEMPEL M., IVANOV V.D., MINNITI D.
	Astron. Astrophys., 569A, 49-49 (2014)
	Confirmation of a galaxy cluster hidden behind the Galactic bulge using the VVV survey.
o	Table 2: <[CAD2014] NN> (Nos 1-15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CAD98]
[CAD98]	(Caldwell+Armandroff+Da Costa+, 1998)
Write:	<<[CAD98] F8D1>> <<[CAD98] BK5N NNNN-N>> <<[CAD98] F8D1 NNNN-N>> <<[CAD98] F8D1-GC1>>
N:	1+13+56+1
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST WFPC2 observations. Table 1: N=1 galaxy, named 'F8D1' (found on 8th field) by the authors. the galaxy 'BK5N' = BK 5N. Table 4: V* in the fields of 'BK5N' and 'F8D1', format 'BK5N NNNN-N' and 'F8D1 NNNN-N', a 4 digit number to which is appended the number N of the CCD chip Table 5: N=1 globular cluster in F8D1, named 'F8D1-GC1'
in source:	NAME M 81 GROUP
in source:	BK 5N
in source:	NAME F8D1
Ref:	=1998AJ....115..535C
by	CALDWELL N. , ARMANDROFF T.E., DA COSTA G.S., SEITZER P.
	Astron. J., 115, 535-558 (1998)
	Dwarf elliptical galaxies in the M81 group: the structure and stellar populations of BK5N and F8D1.
o	p.539, Virgo systems = [IBM88] V2L8 and V3L1.
o	Table 1: <[CAD98] F8D1> = <NAME F8D1>. Table 4: <[CAD98] BK5N NNNN-N> N=13, <[CAD98] F8D1 NNNN-N> N=56. Table 5: <[CAD98] F8D1-GC1> = <NAME F8D1-GC1>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CADIS
CADIS	(Calar Alto Deep Imaging Survey)
Write:	<<CADIS HH-xxxyyy>> <<CADIS FF-LMSN>> <<CADIS FF-ERON>>
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	'HH-xxxyyy' is the generic format of the survey, given by the authors. 'HH' is the field number (e.g. 09 or 16) and xxx as well as yyy are coordinates in arcseconds relative to the field centers. 'LMS' are Low Mass Stars. 'ERO' are Extremely Red Objects. See also [WMT98], [TBF99], [WMR99].
Ref:	=1998A&A...338..127W
by	WOLF C. , MUNDT R., THOMPSON D., CHAFFEE F., BECKWITH S.V.W., FOCKENBROCK R., FRIED J., HIPPELEIN H., HUANG J.-S., VON KUHLMANN B., LEINERT C., MEISENHEIMER K., PHLEPS S., ROESER H.-J., THOMMES E.
	Astron. Astrophys., 338, 127-131 (1998)
	Discovery of three very distant M and L dwarfs.
o	Table 1: <[WMT98] FF-LMSN> = <CADIS FF-LMSN> = <CADIS FF-xxxyyy>, N=3.
Ref:	=1999A&A...343..399W
by	WOLF C. , MEISENHEIMER K., ROESER H.-J., BECKWITH S.V.W., FOCKENBROCK R., HIPPELEIN H., VON KUHLMANN B., PHLEPS S., THOMMES E.
	Astron. Astrophys., 343, 399-406 (1999)
	Did most high-redshift quasars escape detection?
o	Table 2: <[WMR99] HHh-NNNN> = <CADIS FF-xxxyyy>, N=23.
Ref:	=2004A&A...418..475M
by	MAIER C. , MEISENHEIMER K., HIPPELEIN H.
	Astron. Astrophys., 418, 475-485 (2004)
	The metallicity-luminosity relation at medium redshift based on faint CADIS emission line galaxies.
o	Table 2: <CADIS HH-NNNNNN> N=18.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CADIS
CADIS	(Calar Alto Deep Imaging Survey)
*****	Avoid the usage of CADIS, prefer [MMT2003]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CADIS
CADIS	(Calar Alto Deep Imaging Survey)
*****	Avoid the usage of CADIS, prefer [TBF99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CADIS
CADIS	(Calar Alto Deep Imaging Survey)
*****	Avoid the usage of CADIS, prefer [WMR99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CADIS
CADIS	(Calar Alto Deep Imaging Survey)
*****	Avoid the usage of CADIS, prefer [WMT98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CAE99]
[CAE99]	(Crawford+Allen+Ebeling+, 1999)
Write:	<<[CAE99] ACO NNNN>> <<[CAE99] ACO NNNN a>> <<[CAE99] ACO NNNNa>> <<[CAE99] ACO NNNNa a>> <<[CAE99] Z NNNN>> <<[CAE99] Z NNNN a>> <<[CAE99] RX JHHMM.m+DDMM>> <<[CAE99] RX JHHMM.m+DDMM a>> <<[CAE99] RX JHHMM.m+DDMM W>>
N:	254+38
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	New spectra of dominant galaxies in X-ray clusters: Tables 1, 2: N=254 G in 215 clusters. Table 3: N=38 G in 27 clusters for which the authors have not observed the dominant galaxies, but used literature to identified the possible galaxies. In the format, galaxies are identified by the name of their host cluster, followed by the letter a, b, ... when more than one galaxy in the same cluster. See also [AEF92], [CEF95].
Ref:	=1999MNRAS.306..857C
by	CRAWFORD C.S. , ALLEN S.W., EBELING H., EDGE A.C., FABIAN A.C.
	Mon. Not. R. Astron. Soc., 306, 857-896 (1999)
	The ROSAT Brightest Cluster Sample - III. Optical spectra of the central cluster galaxies.
o	Tables 1, 2, 3: <[CAE99] ACO NNNN>, <[CAE99] ACO NNNN a>, <[CAE99] ACO NNNNa>, <[CAE99] ACO NNNNa a>, <[CAE99] Z NNNN>, <[CAE99] Z NNNN a>, <[CAE99] RX JHHMM.m+DDMM>, <[CAE99] RX JHHMM.m+DDMM a>, <[CAE99] RX JHHMM.m+DDMM W>, N=213+41+38.
=E=	Catalogue in electronic form as <J/MNRAS/306/857/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CaFS
CaFS	(Case univ., A and F *)
*****	Avoid the usage of CaFS, prefer Case A-F
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [CAH2008]
[CAH2008]	(Chavarria+Allen+Hora+, 2008)
Write:	<<[CAH2008] DD.dddddd+DD.ddddd>> <<[CAH2008] JHHMMSS.s+DDMMSS.s>> <<[CAH2008] GLLL.ll+B.bb>>
N:	510+5+7
Object:	YSO + * + Cluster of * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Spitzer IRAC, NOAO 2.1m Flamingos, Keck NIRC, and FCRAO SEQUOIA observations of the star-forming complex Sh 2-254-Sh 2-258. Search for YSOs.
in source:	SH 2-254
in source:	SH 2-255
in source:	SH 2-256
in source:	SH 2-257
in source:	SH 2-258
Ref:	=2008ApJ...682..445C
by	CHAVARRIA L.A. , ALLEN L.E., HORA J.L., BRUNT C.M., FAZIO G.G.
	Astrophys. J., 682, 445-462 (2008)
	Spitzer observations of the massive star-forming complex S254-S258: structure and evolution.
o	Table 3, col. "Catalog Name": HD 253237 is a msiprint for HD 253327; ALS 19 and HD 253327 should be switched (to match the correct HII region).
o	Table 2: <[CAH2008] DD.dddddd+DD.ddddd> N=510. Table 3: <[CAH2008] JHHMMSS.s+DDMMSS.s> N=5. Table 4, Fig.12: <[CAH2008] GLLL.ll+B.bb> N=7.
=E=	Catalogue in electronic form as <J/ApJ/682/445/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CAHA
CAHA	(Quanz+Goldman+Henning+, 2010) (Not yet in Simbad)
*****	Avoid the usage of CAHA, prefer [QGH2010]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CAI86]
[CAI86]	(Cook+Aaronson+Illingworth, 1986)
Write:	<<[CAI86] VN>>
N:	2
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Stat:	is completely incorporated in Simbad
Note:	Two new Cepheids were discovered (but not numbered) by Cohen, in 1993, BAAS vol. 25, p. 818
in source:	M 101 = NGC 5457
Ref:	=1986ApJ...301L..45C
by	COOK K.H. , AARONSON M., ILLINGWORTH G.
	Astrophys. J., 301, 45-48 (1986)
	Discovery of Cepheids in M 101.
o	[CAI86] V1 = [KIF96] C9, [CAI86] V2 = [KIF96] C5
o	<[CAI86] VN> (Nos V1-V2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CAIRNS
CAIRNS	(Cluster and Infall Region Nearby Survey)
Write:	<<CAIRNS JHHMMSS.ss+DDMMSS.s>>
N:	15654
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	FLWO observations. CAIRNS is a spectroscopic survey of the infall regions surrounding 8 nearby clusters of galaxies.
in source:	ACO 119
in source:	ACO 168
in source:	ACO 496
in source:	ACO 539
in source:	ACO 576
in source:	ACO 1367
in source:	ACO 1656 = Coma Cluster
in source:	ACO 2199
in source:	ACO 194
Ref:	=2003AJ....126.2152R
by	RINES K. , GELLER M.J., KURTZ M.J., DIAFERIO A.
	Astron. J., 126, 2152-2170 (2003)
	CAIRNS: the cluster and infall region nearby survey. I. Redshifts and mass profiles.
o	Tables 3-8: <CAIRNS JHHMMSS.ss+DDMMSS.s> N=19796.
=E=	Catalogue in electronic form as J/AJ/126/2152
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CAK2018]
[CAK2018]	(Cariddi+Azatyan+Kurfurst+, 2018)
Write:	<<[CAK2018] NNN>>
N:	150
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	ESO 3.6m telescope EFOSC2 observations of N=150 stars in the field of the open cluster Hogg 16.
in source:	C 1326-609 = Cl Hogg 16
Ref:	=2018NewA...58....1C
by	CARIDDI S. , AZATYAN N.M., KURFURST P., STOFANOVA L., NETOPIL M., PAUNZEN E., PINTADO O.I., AIDELMAN Y.J.
	NewA, 58, 1-9 (2018)
	A search for peculiar stars in the open cluster Hogg 16.
o	In the abstract CD-60 4703 is a misprint for CPD-60 4703
o	Table 4: <[CAK2018] NNN> (Nos 1-150).
=E=	Catalogue in electronic form as <J/other/NewA/58.1/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CAL
CAL	(Columbia Astrophys. Laboratory)= (LHG)
Write:	<<CAL NN>> <<CAL A>>
N:	97+5
Object:	(Soft X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	1981ApJ...248..925L: (Nos 1-97), Map 1984ApJ...286..196C: sources not detected in the original IPC survey of CAL, (Nos A-G). Sources C and D are marginal unconfirmed HRI detections. See LMC X
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1981ApJ...248..925L
by	LONG K.S. , HELFAND D.J., GRABELSKY D.A.
	Astrophys. J., 248, 925-944 (1981)
	A soft X-ray study of the Large Magellanic Cloud.
o	Table 2: <CAL NN> (Nos 1-97)
Ref:	=1984ApJ...286..196C
by	COWLEY A.P. , CRAMPTON D., HUTCHINGS J.B., HELFAND D.J., HAMILTON T.T., THORSTENSEN J.R., CHARLES P.A.
	Astrophys. J., 286, 196-208 (1984)
	Optical counterparts of the Large Magellanic Cloud X-ray point sources.
o	Table 1: <CAL A> (Nos A-G), Nos C and D missing. Fig.2: <[CCH84] CAL NN Star N>, <[CCH84] CAL A Star N>, N=17.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Calan
Calan	(Calan obs.)
*****	Avoid the usage of Calan, prefer Ser
Details on Acronym: Calar Alto
Calar Alto	(Calar Alto obs.)
*****	Avoid the usage of Calar Alto, prefer [WEB76]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Caldwell
Caldwell	(Caldwell)= (C)
Write:	<<Caldwell NNN>>
N:	109
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Catalog of N=109 deep-sky objects of interest for amateur astronomers, as a complement to the Messier catalog.
Ref:	=1995S&T....90f..38M
by	MOORE P.
	Sky Telesc., 90, part no 6, 38-None (1995)
	Beyond Messier : the Caldwell catalog.
o	<Caldwell NNN> (Nos 1-109).
o	objects not in SIMBAD (amateur astronomy)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CALYMHA
CALYMHA	(CAlibrating LYMan-α with Hα)
Write:	<<CALYMHA -S16-NNN>>
N:	440
Object:	Line Emitter (SIMBAD class: EmObj = Emission Object)
Note:	INT WFC narrowband observations of N=440 emission line galaxies in the COSMOS and UDS fields, as part of the CAlibrating LYMan-α with Hα (CALIMHA) pilot survey.
in source:	NAME COSMOS Field
Ref:	=2017MNRAS.466.1242S
by	SOBRAL D. , MATTHEE J., BEST P., STROE A., ROTTGERING H., OTEO I., SMAIL I., MORABITO L., PAULINO-AFONSO A.
	Mon. Not. R. Astron. Soc., 466, 1242-1258 (2017)
	The CALYMHA survey: Lyα luminosity function and global escape fraction of Lyα photons at z = 2.23.
o	Table A2: <CALYMHA-S16-NNN> (Nos 1-440).
=E=	Catalogue in electronic form as <J/MNRAS/466/1242/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cam
Cam	(Cambridge survey)
*****	Avoid the usage of Cam, prefer Cambridge
Origin	of the Acronym: L (1997MNRAS.288...78T)
Details on Acronym: Cam
Cam	(Cambresy+)
*****	Avoid the usage of Cam, prefer [CCE98]
Origin	of the Acronym: L (2004ApJ...162..816L)
Details on Acronym: Cam
Cam	(Camelopardalis)
*****	Avoid the usage of Cam, prefer [MWC53]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CAM2005]
[CAM2005]	(Ciroi+Afanasiev+Moiseev+, 2005) (Not yet in Simbad)
Write:	<<[CAM2005] Mrk 315 AN>>
N:	2+1+3+2
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Note:	VATT of the Vatican Observatory (Arizona, USA) photometric and spectroscopic observations of Mrk 315. Filaments (F1, F2), Nucleus (N), quasi-ring structures (A1 to A3), and regions around the nucleus (J1 and J2) are observed.
in source:	Mrk 315
Ref:	=2005MNRAS.360..253C
by	CIROI S. , AFANASIEV V.L., MOISEEV A.V., BOTTE V., MILLE F.D., DODONOV S.N., RAFANELLI P., SMIRNOVA A.A.
	Mon. Not. R. Astron. Soc., 360, 253-271 (2005)
	New photometric and spectroscopic observations of the Seyfert galaxy Mrk 315.
o	Text: <[CAM2005] Mrk 315 AN> (Nos F1-F2, N, A1-A3, J1-J2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Camargo
Camargo	(Camargo)
Write:	<<Camargo NNNN>>
N:	1109 (SIMBAD class: Cluster*_Candidate = Cluster of Stars Candidate)
Note:	N=1109 open cluster candidates near the Galactic plane. Use of WISE image Atlas.
Ref:	=2015NewA...34...84C
by	CAMARGO D. , BICA E., BONATTO C.
	NewA, 34, 84-97 (2015)
	New Galactic embedded clusters and candidates from a WISE Survey.
o	Table 1: <Camargo NNN> (Nos 1-437).
o	Table 2: objects Majaess NNN, de Wit 2, MLG NN are not in SIMBAD.
Ref:	=2015MNRAS.448.1930C
by	CAMARGO D. , BICA E., BONATTO C., SALERNO G.
	Mon. Not. R. Astron. Soc., 448, 1930-1936 (2015)
	Discovery of two embedded clusters with WISE in the high Galactic latitude cloud HRK 81.4-77.8.
o	Table 1: <Camargo NNN> (Nos 438-439) added.
Ref:	=2015MNRAS.450.4150C
by	CAMARGO D. , BONATTO C., BICA E.
	Mon. Not. R. Astron. Soc., 450, 4150-4160 (2015)
	Tracing the Galactic spiral structure with embedded clusters.
o	Table 1: <Camargo NNN> (Nos 440-446) added.
Ref:	=2016MNRAS.455.3126C
by	CAMARGO D. , BICA E., BONATTO C.
	Mon. Not. R. Astron. Soc., 455, 3126-3135 (2016)
	Characterizing star cluster formation with WISE: 652 newly found star clusters and candidates.
o	Table 1: <Camargo NNNN> (Nos 447-1098) added.
Ref:	=2016A&A...593A..95C
by	CAMARGO D. , BICA E., BONATTO C.
	Astron. Astrophys., 593A, 95-95 (2016)
	New detections of embedded clusters in the Galactic halo.
o	Tables 1-2: <Camargo NNNN> (Nos 1099-1101) added.
Ref:	=2018ApJ...860L..27C
by	CAMARGO D.
	Astrophys. J., 860L, 27-27 (2018)
	Five new globular clusters discovered in the Galactic bulge.
o	Table 1: <Camargo NNNN> (Nos 1102-1106) added.
Ref:	=2019MNRAS.484L..90C
by	CAMARGO D. , MINNITI D.
	Mon. Not. R. Astron. Soc., 484L, 90-94 (2019)
	Three candidate globular clusters discovered in the Galactic bulge.
o	<Camargo NNNN> (Nos 1107, 1108, 1109) added.
=E=	Catalogue in electronic form as J/other/NewA/34.84
=E=	Catalogue in electronic form as <J/MNRAS/455/3126/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Cambridge
Cambridge	(Cambridge survey)= (C) = (Cam)
Write:	<<Cambridge HHMM+DDd>> <<Cambridge HHMM+DDMMW>> <<Cambridge HH-NNA>>
Object:	HII G (SIMBAD class: HIIG = HII Galaxy)
Note:	HII galaxies from a Cambridge survey of Hazard C., 1985. First references with Cambridge objects.
Ref:	=1986MNRAS.223..811C
by	CAMPBELL A. , TERLEVICH R., MELNICK J.
	Mon. Not. R. Astron. Soc., 223, 811-825 (1986)
	The stellar populations and evolution of HII galaxies - I. High signal-to-noise optical spectroscopy.
o	Table 1: <Cambridge HHMM+DDd> N=5, <Cambridge HH-NNA> N=1.
Ref:	=1988MNRAS.235..297M
by	MELNICK J. , TERLEVICH R., MOLES M.
	Mon. Not. R. Astron. Soc., 235, 297-313 (1988)
	Giant H II regions as distance indicators- II. Application to H II galaxies and the value of the Hubble constant.
o	Table 1: <Cambridge HHMM+DDMM> N=2 added, <Cambridge HH-NN> N=1 added.
Ref:	=1997MNRAS.288...78T
by	TELLES E. , MELNICK J., TERLEVICH R.
	Mon. Not. R. Astron. Soc., 288, 78-107 (1997)
	The morphology of H II galaxies.
o	Table 1: <Cambridge HHMM+DDMMW> N=3 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CAMC
CAMC	(Carlsberg Astr. Meridian Catalogues)
====>	Equivalent to: CMC
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CAN
CAN	(Cluster Assignement Number)
Write:	<<CAN NNN>>
N:	143
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table 5, col(3): cluster assignement number (CAN) for each GIN (col(1)) and [WCB96] (col(2)) galaxy. The CAN numbering 'NN' is the same as the CID original numbering in Paper I, other CAN 'NNN' have a distinguishing third leading digit.
Ref:	=1999MNRAS.305..259W
by	WEGNER G. , COLLESS M., SAGLIA R.P., McMAHAN R.K.Jr, DAVIES R.L., BURSTEIN D., BAGGLEY G.
	Mon. Not. R. Astron. Soc., 305, 259-296 (1999)
	The peculiar motions of early-type galaxies in two distant regions - II. The spectroscopic data.
o	Table 5, col(3): <CAN NNN> N=143 among (Nos 1-356).
=E=	Catalogue in electronic form as J/MNRAS/305/259
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CANDELS COSMOS F160W
CANDELS COSMOS F160W	(CANDELS COSMOS source detected in the HST/F160W-band)
Write:	<<CANDELS COSMOS F160W JHHMMSS.ss+DDMMSS.s>>
Object:	Star + Galaxy (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	The catalog is a F160W-selected hot+cold catalog covering about 216 sq arcmin, containing 38671 sources. Photometry is available for ugriz* (CFHT), Bg+Vr+i+z+ (Subaru), CANDELS ACS (F606W, F814W), CANDELS WFC3 (F125W, F160W), YJHKs UltraVISTA, Spitzer IRAC (3.6, 4.5, 5.8 and 8.0um) along with medium and narrow band data by NEWFIRM (J1J2J3H1H2K) and Subaru (14 bands). We also provide some spectroscopic redhsifts available for a few number of sources as well as additional parameters such as SExtractor morphology parameters. To appear in the ApJS.
Notes:	The same acronym has been approved for the CANDELS UDS and GOODS-S catalogs published in Galametz+ (2013ApJS..206...10G) and Guo+ (2013ApJS..207...24G) respectively.
Ref:	=2017ApJS..228....7N
by	NAYYERI H. , HEMMATI S., MOBASHER B., FERGUSON H.C., COORAY A., BARRO G., FABER S.M., DICKINSON M., KOEKEMOER A.M., PETH M., SALVATO M., ASHBY M.L.N., DARVISH B., DONLEY J., DURBIN M., FINKELSTEIN S., FONTANA A., GROGIN N.A., GRUETZBAUCH R., HUANG K., KHOSTOVAN A.A., KOCEVSKI D., KODRA D., LEE B., NEWMAN J., PACIFICI C., PFORR J., STEFANON M., WIKLIND T., WILLNER S.P., WUYTS S., CASTELLANO M., CONSELICE C., DOLCH T., DUNLOP J.S., GALAMETZ A., HATHI N.P., LUCAS R.A., YAN H.
	Astrophys. J., Suppl. Ser., 228, 7-7 (2017)
	CANDELS multi-wavelength catalogs: source identification and photometry in the CANDELS COSMOS Survey Field.
o	Table 9, col(1): <[NHM2017] NNNNN> (Nos 1-38671) = Table 9, col(2): <CANDELS COSMOS F160W JHHMMSS.ss+DDMMSS.s> N=38671. University of California Irvine
=E=	Catalogue in electronic form as <J/ApJS/228/7/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CANDELS EGS F160W
CANDELS EGS F160W	(CANDELS EGS source detected in the HST/F160W-band)
Write:	<<CANDELS EGS F160W JHHMMSS.s+DDMMSS.s>>
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	0.4-8µm multi-wavelength photometric catalog of N=41457 F160W-sources in the Extended Groth Strip (EGS) field, built on the Hubble Space Telescope (HST) WFC3 and ACS data from the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS), and it incorporates the existing HST data from the All-wavelength Extended Groth strip International Survey (AEGIS) and the 3D-HST program. See also [SYM2017]. See also CANDELS UDS F160W and [GGF2013] in the UKIDSS Ultra Deep Survey field. See also CANDELS GDS F160W and [GFG2013b] in the GOODS South field.
in source:	NAME Extended Groth Strip
Ref:	=2017ApJS..229...32S
by	STEFANON M. , YAN H., MOBASHER B., BARRO G., DONLEY J.L., FONTANA A., HEMMATI S., KOEKEMOER A.M., LEE B., LEE S.-K., NAYYERI H., PETH M., PFORR J., SALVATO M., WIKLIND T., WUYTS S., ASHBY M.L.N., CASTELLANO M., CONSELICE C.J., COOPER M.C., COORAY A.R., DOLCH T., FERGUSON H., GALAMETZ A., GIAVALISCO M., GUO Y., WILLNER S.P., DICKINSON M.E., FABER S.M., FAZIO G.G., GARDNER J.P., GAWISER E., GRAZIAN A., GROGIN N.A., KOCEVSKI D., KOO D.C., LEE K.-S., LUCAS R.A., McGRATH E.J., NANDRA K., NEWMAN J.A., VAN DER WEL A.
	Astrophys. J., Suppl. Ser., 229, 32-32 (2017)
	CANDELS multi-wavelength catalogs: source identification and photometry in the CANDELS Extended Groth Strip.
o	Table 6, col(1): <[SYM2017] NNNNN> (Nos 1-41457) = Table 6, col(2): <CANDELS EGS F160W JHHMMSS.s+DDMMSS.s> N=41457.
=E=	Catalogue in electronic form as <J/ApJS/229/32/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CANDELS GDN
CANDELS GDN	(CANDELS GDN source detected in the HST/F160W-band)
Write:	<<CANDELS GDN JHHMMSS.s+DDMMSS.s>>
N:	35445
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	A WFC3 F160W (H-band) selected catalog in the CANDELS/GOODS-N field containing photometry from the ultraviolet (UV) to the far-infrared (IR), photometric redshifts, and stellar parameters derived from the analysis of the multiwavelength data. The catalog contains N=35445 sources over the 171 arcmin2 of the CANDELS F160W mosaic. For more information, visit https://archive.stsci.edu/prepds/candels/ See also [GFG2013b]. See also CANDELS UDS F160W, CANDELS EGS F160W, <%M CANDELS GDS F160W>, CANDELS UDS F160W.
in source:	NAME GOODS North Field
Ref:	=2019ApJS..243...22B
by	BARRO G. , PEREZ-GONZALEZ P.G., CAVA A., BRAMMER G., PANDYA V., ELICHE MORAL C., ESQUEJ P., DOMINGUEZ-SANCHEZ H., ALCALDE PAMPLIEGA B., GUO Y., KOEKEMOER A.M., TRUMP J.R., ASHBY M.L.N., CARDIEL N., CASTELLANO M., CONSELICE C.J., DICKINSON M.E., DOLCH T., DONLEY J.L., BRIONES N.E., FABER S.M., FAZIO G.G., FERGUSON H., FINKELSTEIN S., FONTANA A., GALAMETZ A., GARDNER J.P., GAWISER E., GIAVALISCO M., GRAZIAN A., GROGIN N.A., HATHI N.P., HEMMATI S., HERNAN-CABALLERO A., KOCEVSKI D., KOO D.C., KODRA D., LEE K.-S., LIN L., LUCAS R.A., MOBASHER B., McGRATH E.J., NANDRA K., NAYYERI H., NEWMAN J.A., PFORR J., PETH M., RAFELSKI M., RODRIGUEZ-MUNOZ L., SALVATO M., STEFANON M., VAN DER WEL A., WILLNER S.P., WIKLIND T., WUYTS S.
	Astrophys. J., Suppl. Ser., 243, 22-22 (2019)
	The CANDELS/SHARDS multiwavelength catalog in GOODS-N: photometry, photometric redshifts, stellar masses, emission-line fluxes, and star formation rates.
o	<CANDELS GDN JHHMMSS.s+DDMMMSS.s> N=35445 = <[BPC2019] NNNNN> N=35445 among (Nos 1-35451).
=E=	Catalogue in electronic form as <J/ApJS/243/22/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CANDELS GDS F160W
CANDELS GDS F160W	(CANDELS GDS source detected in the HST/F160W-band)
Write:	<<CANDELS GDS F160W JHHMMSS.ss+DDMMSS.s>>
N:	34930
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	UV to mid-infrared multi-wavelength catalog in the CANDELS GOODS-South field, combining newly obtained CANDELS HST WFC3 F105W, F125W, and F160W data with existing public data. The catalog of N=34930 sources is based on source detection in the WFC F160W band. See also [GFG2013b]. See also CANDELS UDS F160W and [GGF2013] in the UKIDSS Ultra Deep Survey field.
in source:	NAME GOODS South Field
Ref:	=2013ApJS..207...24G
by	GUO Y. , FERGUSON H.C., GIAVALISCO M., BARRO G., WILLNER S.P., ASHBY M.L.N., DAHLEN T., DONLEY J.L., FABER S.M., FONTANA A., GALAMETZ A., GRAZIAN A., HUANG K.-H., KOCEVSKI D.D., KOEKEMOER A.M., KOO D.C., McGRATH E.J., PETH M., SALVATO M., WUYTS S., CASTELLANO M., COORAY A.R., DICKINSON M.E., DUNLOP J.S., FAZIO G.G., GARDNER J.P., GAWISER E., GROGIN N.A., HATHI N.P., HSU L.-T., LEE K.-S., LUCAS R.A., MOBASHER B., NANDRA K., NEWMAN J.A., VAN DER WEL A.
	Astrophys. J., Suppl. Ser., 207, 24 (2013)
	CANDELS multi-wavelength catalogs: source detection and photometry in the GOODS-south field.
o	catalog.dat: <[GFG2013b] NNNNN> (Nos 1-34930) = <CANDELS GDS F160W JHHMMSS.ss+DDMMSS.s> N=34930.
=E=	Catalogue in electronic form as J/ApJS/207/24
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CANDELS UDS F160W
CANDELS UDS F160W	(CANDELS UDS source detected in the HST/F160W-band)
Write:	<<CANDELS UDS F160W JHHMMSS.ss+DDMMSS.s>>
N:	35932
Note:	The catalog is a F160W-selected hot+cold catalog covering about 200 sq arcmin, containing 35932 sources. Photometry is available for U (CFHT), BVRci'z' (Subaru), CANDELS ACS (F606W,F814W), CANDELS WFC3 (F125W, F160W), HAWK-i YKs, UKIDSS JHK (DR8), Spitzer IRAC SEDS (3.6, 4.5um) and SpUDS (3.6, 4.5, 5.8, 8.0um). We also provide some spectroscopic redhsifts available for a few number of sources as well as additional parameters such as SExtractor morphology parameters... The catalog will be available simultaneously to the scientific community on the official CANDELS website. See also [GGF2013]. See also CANDELS GDS F160W and [GFG2013b] in the GOODS-South field.
Ref:	=2013ApJS..206...10G
by	GALAMETZ A. , GRAZIAN A., FONTANA A., FERGUSON H.C., ASHBY M.L.N., BARRO G., CASTELLANO M., DAHLEN T., DONLEY J.L., FABER S.M., GROGIN N., GUO Y., HUANG K.-H., KOCEVSKI D.D., KOEKEMOER A.M., LEE K.-S., McGRATH E.J., PETH M., WILLNER S.P., ALMAINI O., COOPER M., COORAY A., CONSELICE C.J., DICKINSON M., DUNLOP J.S., FAZIO G.G., FOUCAUD S., GARDNER J.P., GIAVALISCO M., HATHI N.P., HARTLEY W.G., KOO D.C., LAI K., DE MELLO D.F., McLURE R.J., LUCAS R.A., PARIS D., PENTERICCI L., SANTINI P., SIMPSON C., SOMMARIVA V., TARGETT T., WEINER B.J., WUYTS S., (The CANDELS Team)
	Astrophys. J., Suppl. Ser., 206, 10 (2013)
	CANDELS multiwavelength catalogs: source identification and photometry in the CANDELS UKIDSS ultra-deep survey field.
o	Table 3: <[GGF2013] NNNNN> (Nos 1-35932) = <CANDELS UDS F160W JHHMMSS.ss+DDMMSS.s> N=35932. INAF - Observatory of Rome
=E=	Catalogue in electronic form as J/ApJS/206/10
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CAP
CAP	(Catalog of Pantoja)
Write:	<<CAP HHMM+DDa>>
N:	369
Object:	G (SIMBAD class: Galaxy)
Note:	N=369 galaxies from the 'CAP' catalog (Pantoja 1995 thesis)
Ref:	=1997AJ....113..905P
by	PANTOJA C.A. , ALTSCHULER D.R., GIOVANARDI C., GIOVANELLI R.
	Astron. J., 113, 905-936 (1997)
	21-cm line observations of galaxies in the zone of avoidance.
o	T.2: a100 = UGCA 100
o	Table 1: <CAP HHMM+DDa> N=369
=E=	Catalogue in electronic form as J/AJ/113/905
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CAP2014]
[CAP2014]	(Cantalupo+Arrigoni-Battaia+Prochaska+, 2014)
Write:	<<[CAP2014] UM 287 nebula>> <<[CAP2014] UM 287b>>
N:	1+1
Object:	Lyman Alpha Nebula + QSO (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Keck-I LRIS observations of N=1 Lyman α nebula and N=1 companion quasar in the field of the radio-quiet quasar UM 287.
Ref:	=2014Natur.506...63C
by	CANTALUPO S. , ARRIGONI-BATTAIA F., PROCHASKA X., HENNAWI J.F., MADAU P.
	Natur, 506, 63-66 (2014)
	A cosmic web filament revealed in Lyman-{alf} emission around a luminous high-redshift quasar.
o	Fig. 2: <[CAP2014] UM 287 nebula> = <NAME Slug Nebula>. Fig. 2: <[CAP2014] UM 287b> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CaPa
CaPa	(Caloi+Panagia)= CiPg (Not yet in Simbad)
Write:	<<CaPa N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	= PK 065-27 2, rejected as PN in 1992, Acker+ catalog
Ref:	=1974A&A....36..139C
by	CALOI V. , PANAGIA N.
	Astron. Astrophys., 36, 139-141 (1974)
	On the nature of the 10 micron source in M 15.
Details on Acronym: Car
Car	(Carina)
*****	Avoid the usage of Car, prefer [ABC89]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Car
Car	(Carina)
*****	Avoid the usage of Car, prefer [MWC53]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Car
Car	(Carina)
*****	Avoid the usage of Car, prefer [VMF2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CAR2008]
[CAR2008]	(Carrasco-Gonzalez+Anglada+Rodriguez+, 2008)
Write:	<<[CAR2008] VLA 2Aa>> <<[CAR2008] wN>>
N:	4+2+6
Object:	Poss. YSO + (Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA 3.6cm and 7mm observations of the core of LDN 723: N=4 YSO candidates associated with [AER91] 2, VLA 2C shows 2 peaks Ca and Cb. N=6 radio continuum knots are also detected (wn).
in source:	LDN 723
Ref:	=2008ApJ...676.1073C
by	CARRASCO-GONZALEZ C. , ANGLADA G., RODRIGUEZ L.F., TORRELLES J.M., OSORIO M., GIRART J.M.
	Astrophys. J., 676, 1073-1081 (2008)
	A multiple system of radio sources at the core of the L723 multipolar outflow.
o	Figs 1-3, Table 3: <[CAR2008] VLA 2Aa> (Nos A-D, 2Ca, 2Cb). Fig. 1: <[CAR2008] wN> (Nos w1-w2, e1-e2, n1, s1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CAR83]
[CAR83]	(Cohen+Aitken+Roche+, 1983)
Write:	<<[CAR83] PP 13N>> <<[CAR83] PP 13S>> <<[CAR83] PP 13S IRS>>
N:	3
Object:	Part of Nebula (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Fig 1: Two components are well-separated in PP 13, the southern is a very red nebula, containing an infrared source, the northern object is stellar and quite faint. See also [SA98].
in source:	PP 13
Ref:	=1983ApJ...273..624C
by	COHEN M. , AITKEN D.K., ROCHE P.F., WILLIAMS P.M.
	Astrophys. J., 273, 624-632 (1983)
	The unique cometary nebula Parsamian 13.
o	Parsamian 13 = PP 13 in SIMBAD
o	Fig 1: <[CAR83] PP 13N>, <[CAR83] PP 13S>, <[CAR83] PP 13S IRS>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CARLA
CARLA	(Clusters Around Radio-Loud AGN)
Write:	<<CARLA JHHMM+DDMM>>
N:	about 420 (SIMBAD class: ClG = Cluster of Galaxies)
Note:	The CARLA project has used 400 hours of Spitzer time to image 420 high-redshift radio-loud AGN, searching for associated galaxy clusters (CARLA = Clusters Around Radio-Loud AGN). That work is reported in Wylezalek et al. (2013, 2014). Our follow-up 40 orbit Hubble program is starting to confirm some of these clusters, and our desire is to use the "CARLA" designation for spectroscopically confirmed clusters. The first spectroscopic confirmation is submitted, and the next set of two papers should be submitted this month. We are also doing ground-based follow-up using a variety of telescopes (i.e., Keck, VLT, Palomar, ....). Wylezalek et al. (2013ApJ...769...79W, 2014ApJ...786...17W) Cooke et al. (submitted); Noirot et al. (in prep.); Rettura et al. (in prep.)
Notes:	The actual source coordinates listed above are for the target radio-loud AGN, but the AGN isn't always exactly at the cluster center (nor is it always obvious to identify the center of a young, forming cluster). Thus our desire to use the HHMM+DDMM format rather than something more exact.
Auth.:	Daniel Stern Jet Propulsion Laboratory/California Institute of Technology
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: Cas
Cas	(Cassiopeia)
*****	Avoid the usage of Cas, prefer [MWC53]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Cas
Cas	(Cassiopeia)
Write:	<<NAME Cas N>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Ref:	=1995A&A...293L..33H
by	HUCHTMEIER W.K. , LERCHER G., SEEBERGER R., SAURER W., WEINBERGER R.
	Astron. Astrophys., 293, 33-36 (1995)
	Two new possible members of the IC342-Maffei1/2 group of galaxies.
o	<NAME Cas N> (Nos 1-2)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cas1
Cas1	(Cassiopeia OB 1)
*****	Avoid the usage of Cas1, prefer Glazar
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cas2
Cas2	(Cassiopeia OB 2)
*****	Avoid the usage of Cas2, prefer Glazar
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CAS2006]
[CAS2006]	(Castro-Tirado+Anupama+Srividya+, 2006)
Write:	<<[CAS2006] A>>
N:	4
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Search for optical counterparts of GRB 060801.
Ref:	=2006GCN..5384....1C
by	CASTRO-TIRADO A.J. , ANUPAMA G.C., SRIVIDYA S., RAMYA S., DE UGARTE POSTIGO A., SANCHEZ S., MONTOYA L., CASTILLO A., MUNOZ-MATEOS J.C., JELINEK M., GOROSABEL J.
	GRB Coordinates Network, Circular Service, 5384, 1-None (2006)
	GRB 060801: optical observations at hanle and calar alto.
o	<[CAS2006] A> (Nos A-B).
Ref:	=2006GCN..5386....1P
by	PIRANOMONTE S. , COVINO S., MALESANI D., TAGLIAFERRI G., CHINCARINI G., STELLA L.
	GRB Coordinates Network, Circular Service, 5386, 1-None (2006)
	GRB 060801: optical observations at FORS2/VLT.
o	<[CAS2006] A> (Nos C-D) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Case
Case	(Case univ.)= (C) = (NB)
Write:	<<Case NNN>>
N:	749
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Ref:	=1954ApJ...120..129N
by	NASSAU J.J. , BLANCO V.M.
	Astrophys. J., 120, 129-138 (1954)
	Carbon stars at the galactic equator in a zone 4 ° wide.
o	Tables 1a, 1b: <Case NNN> (Nos 1-271)
Ref:	=1957ApJ...125..195N
by	NASSAU J.J. , BLANCO V.M.
	Astrophys. J., 125, 195-208 (1957)
	Carbon stars in two northern Milky Way zones.
o	Tables 1, 2: <Case NNN> (Nos 272-693)
Ref:	=1958ApJ...127..191B
by	BLANCO V.M.
	Astrophys. J., 127, 191-193 (1958)
	Carbon stars at intermediate galactic latitudes.
o	Tables 1a, 1b: <Case NNN> (Nos 694-749)
Details on Acronym: Case
Case	(Case univ.)= (C)
Write:	<<NAME Case N>>
N:	3
Object:	WD (SIMBAD class: WhiteDwarf = White Dwarf)
Ref:	=1960PASP...72..387S
by	STEPHENSON C.B.
	Publ. Astron. Soc. Pac., 72, 387-392 (1960)
	A spectroscopic search for white dwarfs in the Ursa Major cluster.
o	Table I: <NAME Case 1>
Ref:	=1962PASP...74..210S
by	STEPHENSON C.B.
	Publ. Astron. Soc. Pac., 74, 210-214 (1962)
	A spectroscopic search for new white dwarfs.
o	Table II: <NAME Case N> (Nos 2-3)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Case
Case	(Case univ.)
*****	Avoid the usage of Case, prefer SP77
Origin	of the Acronym: L (1985ApJ...289..141E)
Details on Acronym: Case A-F
Case A-F	(Case univ., A and F *)= (AF) = (A-F) = (CaFS)
Write:	<<Case A-F NNNN>>
N:	1110
Object:	A-F * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Finding charts
Ref:	=1988ApJS...66..309S
by	SANDULEAK N.
	Astrophys. J., Suppl. Ser., 66, 309-313 (1988)
	The case low-dispersion northern sky survey. VI. A-F stars in a region near the North Galactic Pole.
o	Table 1: <Case A-F NNN> (Nos 1-183)
Ref:	=1989ApJS...71..549P
by	PESCH P. , SANDULEAK N.
	Astrophys. J., Suppl. Ser., 71, 549-558 (1989)
	The case low-dispersion northern sky survey. X. A-F stars in a region at intermediate galactic latitude primarily in Lynx and Leo Minor.
o	(Erratum) Erratum 1996 ApJS 102, p. 435
o	CASE A-F 193 coord., see erratum
o	Table 1: <Case A-F NNN> (Nos 184-723)
Ref:	=1993ApJS...86..453M
by	MacCONNELL D.J. , STEPHENSON C.B., PESCH P.
	Astrophys. J., Suppl. Ser., 86, 453-474 (1993)
	The Case low-dispersion northern sky survey. XIV. A-F stars in a region southern Canes Venatici.
o	SCC objects not in SIMBAD.
o	Table 1: <Case A-F NNN> (Nos 724-1110)
=E=	Catalogue in electronic form as J/ApJS/66/309
=E=	Catalogue in electronic form as J/ApJS/71/549
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CaseG
CaseG	(Case univ., G)
====>	Equivalent to: CasG
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: CasG
CasG	(Case univ., G)= CaseG = (CG)
Write:	<<CasG NNNN>>
N:	1579
Object:	Blue or Em. G (SIMBAD class: Galaxy)
Note:	Identif. charts.
Ref:	=1983ApJS...51..171P
by	PESCH P. , SANDULEAK N.
	Astrophys. J., Suppl. Ser., 51, 171-182 (1983)
	The Case low-dispersion northern sky survey. I.
o	Table 1: <CasG NN> (Nos 1-71), Table 1A: <CasHII Z FFF-NNN a> N=4, Table 2: <CSO NN> (Nos 1-59), Table 3: <CBS NN> (Nos 1-28)
Ref:	=1984ApJS...55..517S
by	SANDULEAK N. , PESCH P.
	Astrophys. J., Suppl. Ser., 55, 517-532 (1984)
	The Case low-dispersion northern sky survey. II.
o	(Erratum) Erratum 1996 ApJS 103, p. 513
o	Table 1: <CasG NNN> (Nos 72-196), Table 1A: <CasHII Z FFF-NNN a> N=40, Table 2: <CSO NNN> (Nos 60-179), Table 3: <CBS NN> (Nos 29-66)
Ref:	=1986ApJS...60..543P
by	PESCH P. , SANDULEAK N.
	Astrophys. J., Suppl. Ser., 60, 543-549 (1986)
	The Case low-dispersion northern sky survey. III.
o	Table 1: <CasG NNN> (Nos 197-326), Table 1A: <CasHII Z FFF-NNN a> N=6, <CasHII HHMMSS.s+DDMM.m a> N=1, Table 2: <CSO NNN> (Nos 180-252), Table 3: <CBS NNN> (Nos 67-124)
Ref:	=1987ApJS...63..809S
by	SANDULEAK N. , PESCH P.
	Astrophys. J., Suppl. Ser., 63, 809-819 (1987)
	The Case low-dispersion northern sky survey. IV. Galaxies in the Bootes void region.
o	Table 1: <CasG NNN> (Nos 327-752), Table 1A: <CasHII ZFFF-NNN a> N=48, <CasHII HHMMSS.s+DDMM.m a> N=2
Ref:	=1988ApJS...66..297P
by	PESCH P. , SANDULEAK N.
	Astrophys. J., Suppl. Ser., 66, 297-307 (1988)
	The Case low-dispersion northern sky survey. V.
o	Table 1: <CasG NNN> (Nos 753-895), Table 1A: <CasHII Z FFF-NNN a> N=20, <CasHII HHMMSS.s+DDMM.m a> N=3, Table 2: <CSO NNN> (Nos 253-401), Table 3: <CBS NNN> (Nos 125-160)
Ref:	=1989ApJS...70..163P
by	PESCH P. , SANDULEAK N.
	Astrophys. J., Suppl. Ser., 70, 163-171 (1989)
	The Case low-dispersion northern sky survey. VIII. A region centered in southern Bootes.
o	Table 1: <CasG NNN> (Nos 896-907), Table 2: <CSO NNN> (Nos 402-602), Table 3: <CBS NNN> (Nos 161-252)
Ref:	=1989ApJS...70..173S
by	SANDULEAK N. , PESCH P.
	Astrophys. J., Suppl. Ser., 70, 173-179 (1989)
	The Case low-dispersion northern sky survey. IX. A region centered in northern Bootes.
o	Table 1: <CasG NNN> (Nos 908-925), Table 2: <CSO NNN> (Nos 603-765), Table 3: <CBS NNN> (Nos 253-324)
Ref:	=1990ApJS...72..291S
by	SANDULEAK N. , PESH P.
	Astrophys. J., Suppl. Ser., 72, 291-301 (1990)
	The Case low-dispersion northern sky survey. XI. A region near the North Galactic Pole including SA 57.
o	Table 1: <CasG NNNN> (Nos 926-1019), Table 2: <CSO NNN> (Nos 766-881), Table 3: <CBS NNN> (Nos 325-350)
Ref:	=1991ApJS...76.1043P
by	PESCH P. , SANDULEAK N., STEPHENSON C.B.
	Astrophys. J., Suppl. Ser., 76, 1043-1053 (1991)
	The Case low-dispersion northern sky survey. XII. A region in southern Canes Venatici.
o	(Erratum) Erratum 1996 ApJS 102, p. 435, and 1996 ApJS 103, p. 513
o	Table 2: <CasG NNNN> (Nos 1020-1213), Table 3: <CasHII PGC NNNNN>, <CasHII PGC NNNNN a> N=3+12, Table 4: <CSO NNNN> (Nos 882-1038), Table 5: <CBS NNN> (Nos 351-382)
Ref:	=1992ApJS...82..471S
by	STEPHENSON C.B. , PESCH P., MacCONNELL D.J.
	Astrophys. J., Suppl. Ser., 82, 471-487 (1992)
	The case Low-Dispersion Northern Sky Survey. XIII. A region in central Bootes and Corona Borealis.
o	Table 1: <CasG NNNN> (Nos 1214-1351), Table 2:<CasHII PGC NNNNN a> N=4, Table 3: <CSO NNNN> (Nos 1039-1121), Table 4: <CBS NNN> (Nos 383-418)
Ref:	=1995ApJS...98...41P
by	PESCH P. , STEPHENSON C.B., MacCONNELL D.J.
	Astrophys. J., Suppl. Ser., 98, 41-67 (1995)
	The Case low-dispersion northern sky survey. XV. A region in Ursa Major and Canes Venatici.
o	(Erratum) Erratum 1996 ApJS 102, p. 435, and 1996 ApJS 103, p. 513
o	Table 1: <CasG NNNN> (Nos 1352-1579), Table 2: <CasHII PGC NNNNN> <CasHII PGC NNNNN a> <CasHII Anon a> N=7+34+2, Table 4: <CSO NNNN> (Nos 1122-1336), Table 5: <CBS NNN> (Nos 419-465)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CasHII
CasHII	(Case univ., HII)= (PGC) = (ZwG)
Write:	<<CasHII Z FFF-NNN a>> <<CasHII HHMMSS.s+DDMM.m a>> <<CasHII PGC NNNNN a>> <<CasHII Anon a>>
N:	170
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Identif. charts.
Ref:	=1983ApJS...51..171P
by	PESCH P. , SANDULEAK N.
	Astrophys. J., Suppl. Ser., 51, 171-182 (1983)
	The Case low-dispersion northern sky survey. I.
o	Table 1: <CasG NN> (Nos 1-71), Table 1A: <CasHII Z FFF-NNN a> N=4, Table 2: <CSO NN> (Nos 1-59), Table 3: <CBS NN> (Nos 1-28)
Ref:	=1984ApJS...55..517S
by	SANDULEAK N. , PESCH P.
	Astrophys. J., Suppl. Ser., 55, 517-532 (1984)
	The Case low-dispersion northern sky survey. II.
o	(Erratum) Erratum 1996 ApJS 103, p. 513
o	Table 1: <CasG NNN> (Nos 72-196), Table 1A: <CasHII Z FFF-NNN a> N=40, Table 2: <CSO NNN> (Nos 60-179), Table 3: <CBS NN> (Nos 29-66)
Ref:	=1986ApJS...60..543P
by	PESCH P. , SANDULEAK N.
	Astrophys. J., Suppl. Ser., 60, 543-549 (1986)
	The Case low-dispersion northern sky survey. III.
o	Table 1: <CasG NNN> (Nos 197-326), Table 1A: <CasHII Z FFF-NNN a> N=6, <CasHII HHMMSS.s+DDMM.m a> N=1, Table 2: <CSO NNN> (Nos 180-252), Table 3: <CBS NNN> (Nos 67-124)
Ref:	=1987ApJS...63..809S
by	SANDULEAK N. , PESCH P.
	Astrophys. J., Suppl. Ser., 63, 809-819 (1987)
	The Case low-dispersion northern sky survey. IV. Galaxies in the Bootes void region.
o	Table 1: <CasG NNN> (Nos 327-752), Table 1A: <CasHII ZFFF-NNN a> N=48, <CasHII HHMMSS.s+DDMM.m a> N=2
Ref:	=1988ApJS...66..297P
by	PESCH P. , SANDULEAK N.
	Astrophys. J., Suppl. Ser., 66, 297-307 (1988)
	The Case low-dispersion northern sky survey. V.
o	Table 1: <CasG NNN> (Nos 753-895), Table 1A: <CasHII Z FFF-NNN a> N=20, <CasHII HHMMSS.s+DDMM.m a> N=3, Table 2: <CSO NNN> (Nos 253-401), Table 3: <CBS NNN> (Nos 125-160)
Ref:	=1991ApJS...76.1043P
by	PESCH P. , SANDULEAK N., STEPHENSON C.B.
	Astrophys. J., Suppl. Ser., 76, 1043-1053 (1991)
	The Case low-dispersion northern sky survey. XII. A region in southern Canes Venatici.
o	(Erratum) Erratum 1996 ApJS 102, p. 435, and 1996 ApJS 103, p. 513
o	Table 2: <CasG NNNN> (Nos 1020-1213), Table 3: <CasHII PGC NNNNN>, <CasHII PGC NNNNN a> N=3+12, Table 4: <CSO NNNN> (Nos 882-1038), Table 5: <CBS NNN> (Nos 351-382)
Ref:	=1992ApJS...82..471S
by	STEPHENSON C.B. , PESCH P., MacCONNELL D.J.
	Astrophys. J., Suppl. Ser., 82, 471-487 (1992)
	The case Low-Dispersion Northern Sky Survey. XIII. A region in central Bootes and Corona Borealis.
o	Table 1: <CasG NNNN> (Nos 1214-1351), Table 2:<CasHII PGC NNNNN a> N=4, Table 3: <CSO NNNN> (Nos 1039-1121), Table 4: <CBS NNN> (Nos 383-418)
Ref:	=1995ApJS...98...41P
by	PESCH P. , STEPHENSON C.B., MacCONNELL D.J.
	Astrophys. J., Suppl. Ser., 98, 41-67 (1995)
	The Case low-dispersion northern sky survey. XV. A region in Ursa Major and Canes Venatici.
o	(Erratum) Erratum 1996 ApJS 102, p. 435, and 1996 ApJS 103, p. 513
o	Table 1: <CasG NNNN> (Nos 1352-1579), Table 2: <CasHII PGC NNNNN> <CasHII PGC NNNNN a> <CasHII Anon a> N=7+34+2, Table 4: <CSO NNNN> (Nos 1122-1336), Table 5: <CBS NNN> (Nos 419-465)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CASSOWARY
CASSOWARY	(Cambridge Sloan Survey of Wide Arcs)
*****	Avoid the usage of CASSOWARY, prefer CSWA
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Caswell
Caswell	(Caswell)
Write:	<<Caswell OH LLL.lll+BB.bbb>> <<Caswell OH LLL.lll+BB.bbww>> <<Caswell H2O LLL.lll+BB.bbb>> <<Caswell H2O LLL.ll+BB.bbww>> <<Caswell CH3OH LLL.lll+BB.bbb>> <<Caswell CH3OH LLL.ll+BB.bbww>>
Object:	Maser (SIMBAD class: Maser)
Ref:	=1977MNRAS.181..427C
by	CASWELL J.L. , HAYNES R.F., GOSS W.M.
	Mon. Not. R. Astron. Soc., 181, 427-433 (1977)
	New OH masers in the direction of H2O masers.
o	<Caswell H2O LLL.l+B.b> N=7, <Caswell OH LLL.ll+B.bb> N=6, cross-id. -> N=10
Ref:	=1980AuJPh..33..139B
by	BATCHELOR R.A. , CASWELL J.L., GOSS W.M., HAYNES R.F., KNOWLES S.H., WELLINGTON K.J.
	Australian J. Phys., 33, 139-157 (1980)
	Galactic plane H2O masers: a southern survey.
o	<Caswell H2O LLL.ll+B.bb> N=68
Ref:	=1980AuJPh..33..639C
by	CASWELL J.L. , HAYNES R.F., GOSS W.M.
	Australian J. Phys., 33, 639-669 (1980)
	Survey of OH Masers at 1665 and 1667 MHz. I. Galactic longitudes 326 ° to 340 °.
o	<Caswell OH LLL.ll+B.bb> N=40
Ref:	=1981AuJPh..34..333C
by	CASWELL J.L. , HAYNES R.F., GOSS W.M., MEBOLD U.
	Australian J. Phys., 34, 333-355 (1981)
	A southern survey of OH masers at 1612 MHz.
o	Table 1: <Caswell OH LLL.ll+B.bb> N=83
Ref:	=1983AuJPh..36..361C
by	CASWELL J.L. , HAYNES R.F.
	Australian J. Phys., 36, 361-399 (1983)
	Survey of OH masers at 1665 MHz. II. Galactic longitude 340 to the galactic centre.
o	<Caswell OH LLL.ll+B.bb> N=49
Ref:	=1983AuJPh..36..401C
by	CASWELL J.L. , BATCHELOR R.A., FORSTER J.R., WELLINGTON K.J.
	Australian J. Phys., 36, 401-415 (1983)
	H2O Masers in the galactic plane. I.
o	<Caswell H2O LLL.ll+B.bb> N=46
Ref:	=1983AuJPh..36..417C
by	CASWELL J.L. , HAYNES R.F.
	Australian J. Phys., 36, 417-442 (1983)
	Atlas of main-line OH masers in the galactic longitude range 3 to 60.
o	<Caswell OH LLL.ll+B.bb> N=55
Ref:	=1983AuJPh..36..443C
by	CASWELL J.L. , BATCHELOR R.A., FORSTER J.R., WELLINGTON K.J.
	Australian J. Phys., 36, 443-451 (1983)
	New H2O masers associated with main-line OH masers in the galactic longitude range 3 to 60.
o	Table 2: <Caswell OH LLL.ll+B.bb> and <Caswell H2O LLL.ll+B.bb>, N=56+37
Ref:	=1987AuJPh..40..215C
by	CASWELL J.L. , HAYNES R.F.
	Australian J. Phys., 40, 215-238 (1987)
	Survey of OH masers at 1665 MHz. III. Galactic longitudes 233 to 326.
o	<Caswell OH LLL.ll+B.bb> N=24
Ref:	=1989AuJPh..42..331C
by	CASWELL J.L. , BATCHELOR R.A., FORSTER J.R., WELLINGTON K.J.
	Australian J. Phys., 42, 331-344 (1989)
	H2O masers in the galactic plane. II. Longitudes 260 to 326.
o	<Caswell H2O LLL.ll+B.bb> N=53
Ref:	=1989A&A...213..339F
by	FORSTER J.R. , CASWELL J.L.
	Astron. Astrophys., 213, 339-350 (1989)
	The spatial relationship of OH and H2O masers.
o	<Caswell OH LLL.ll+B.bb> and <Caswell H2O LLL.ll+B.bb> N=74
Ref:	=1993MNRAS.260..425C
by	CASWELL J.L. , GARDNER F.F., NORRIS R.P., WELLINGTON K.J., McCUTCHEON W.H., PENG R.S.
	Mon. Not. R. Astron. Soc., 260, 425-436 (1993)
	Methanol masers at 12 GHz.
o	<Caswell CH3OH LLL.ll+B.bb> N=57
Ref:	=1995PASA...12...37C
by	CASWELL J.L. , VAILE R.A., ELLINGSEN S.P.
	Publications - Astron. Soc. Australia, 12, 37-53 (1995)
	Variability of methanol masers.
o	<Caswell CH3OH LLL.ll+B.bb> N=95
Ref:	=1995MNRAS.272...96C
by	CASWELL J.L. , VAILE R.A., ELLINGSEN S.P., WHITEOAK J.B., NORRIS R.P.
	Mon. Not. R. Astron. Soc., 272, 96-138 (1995)
	Galactic methanol masers at 6.6 GHz.
o	<Caswell CH3OH LLL.ll+B.bb> N=115
Ref:	=1995MNRAS.273..328C
by	CASWELL J.L. , VAILE R.A.
	Mon. Not. R. Astron. Soc., 273, 328-346 (1995)
	Excited-state OH masers at 6.035 GHz.
o	<Caswell OH LLL.ll+B.bb> N=72, 52 are new
Ref:	=1995MNRAS.274.1126C
by	CASWELL J.L. , VAILE R.A., ELLINGSEN S.P., NORRIS R.P.
	Mon. Not. R. Astron. Soc., 274, 1126-1152 (1995)
	Galactic methanol masers at 12 GHz.
o	<Caswell CH3OH LLL.ll+B.bb> N=131
Ref:	=1995MNRAS.277..210C
by	CASWELL J.L. , VAILE R.A., FORSTER J.R.
	Mon. Not. R. Astron. Soc., 277, 210-216 (1995)
	Methanol and hydroxyl maser positions.
o	<Caswell CH3OH LLL.ll+B.bb> and <Caswell OH LLL.ll+B.bb> N=35+49
Ref:	=1996MNRAS.279...79C
by	CASWELL J.L.
	Mon. Not. R. Astron. Soc., 279, 79-87 (1996)
	A new survey for 6.6-GHz methanol masers.
o	<Caswell CH3OH LLL.lll+B.bbb> N=57, 21 are new, others have a more precise format
Ref:	=1996MNRAS.283..606C
by	CASWELL J.L.
	Mon. Not. R. Astron. Soc., 283, 606-612 (1996)
	A Galactic Centre survey for 6.6-GHz methanol masers.
o	<Caswell CH3OH LLL.lll+B.bbb> N=23, 18 are new
Ref:	=1998MNRAS.297..215C
by	CASWELL J.L.
	Mon. Not. R. Astron. Soc., 297, 215-235 (1998)
	Positions of hydroxyl masers at 1665 and 1667 MHz.
o	in ref list: Houghton 1995MNRAS.273.1033 instead of 263
o	Table 1: <Caswell OH LLL.lll+BB.bbb> about 50 are new.
Ref:	=1999MNRAS.308..683C
by	CASWELL J.L.
	Mon. Not. R. Astron. Soc., 308, 683-690 (1999)
	OH masers at 1612 and 1720 MHz in star-forming regions.
o	Tables 1, 2: <Caswell OH LLL.lll+BB.bbb> N=2 are new.
Ref:	=2000MNRAS.313..599C
by	CASWELL J.L. , YI J., BOOTH R.S., CRAGG D.M.
	Mon. Not. R. Astron. Soc., 313, 599-616 (2000)
	Methanol masers at 107.0 and 156.6GHz.
o	Table 1: <Caswell CH3OH LLL.lll+BB.bbb> N=26 new.
Ref:	=2001MNRAS.326..805C
by	CASWELL J.L.
	Mon. Not. R. Astron. Soc., 326, 805-820 (2001)
	Maser emission from OH at the 6035-MHz transition.
o	Table 1: <Caswell OH LLL.lll+BB.bbb> N=53.
Ref:	=2004MNRAS.351..279C
by	CASWELL J.L.
	Mon. Not. R. Astron. Soc., 351, 279-284 (2004)
	Molecular masers of OH, methanol and water in NGC 3576, NGC 3603 and RCW 79.
o	Table 1: <Caswell OH LLL.lll+BB.bbb> N=2 added, <Caswell H2O LLL.lll+BB.bbb> N=2 added, <Caswell CH3OH LLL.lll+BB.bbb> N=3 added.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CAT2001]
[CAT2001]	(Colina+Alberdi+Torrelles+, 2001)= ([CAT2001a])
Write:	<<[CAT2001] BHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	Poss. SNR (SIMBAD class: SNRemnant_Candidate = SuperNova Remnant Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=1 probable radio SNR in NGC 7469.
in source:	NGC 7469
Ref:	=2001IAUC.7587....1C
by	COLINA L. , ALBERDI A., TORRELLES J.M., PANAGIA N., WILSON A.S.
	IAU Circ., 7587, 1-None (2001)
	Probable radio supernova in NGC 7469.
o	<[CAT2001] BHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CAT2001a]
[CAT2001a]	(Colina+Alberdi+Torrelles+, 2001)
*****	Avoid the usage of [CAT2001a], prefer [CAT2001]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CAT2001b]
[CAT2001b]	(Colina+Alberdi+Torrelles+, 2001)
Write:	<<[CAT2001b] RN>>
N:	3
Object:	Region (SIMBAD class: Region = Region defined in the Sky)
Stat:	is completely incorporated in Simbad
Note:	N=3 bright star-forming regions circumnuclear of the RSN [CAT2001] B230044.30+083616.2.
in source:	NGC 7469
Ref:	=2001ApJ...553L..19C
by	COLINA L. , ALBERDI A., TORRELLES J.M., PANAGIA N., WILSON A.S.
	Astrophys. J., 553, 19-22 (2001)
	Discovery of a bright radio supernova in the circumnuclear starburst of the luminous infrared Seyfert 1 galaxy NGC 7469.
o	Radio Supernova (RSN) = [CAT2001] B230044.30+083616.2.
o	Fig.1, Table 1: <[CAT2001b] RN> (Nos R1-R3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CAVS
CAVS	(Centaurus A, Variable Star)
Write:	<<CAVS NNN>>
N:	271
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	ESO-MPG 2.2m telescope WFI observations of Cen A.
in source:	Cen A = NGC 5128
Ref:	=2008A&A...478..755D
by	DE JONG J.T.A. , KUIJKEN K.H., HERAUDEAU P.
	Astron. Astrophys., 478, 755-762 (2008)
	Ground-based variability surveys towards Centaurus A: worthwhile or not?
o	Table 3: <CAVS NNN> (Nos 1-271).
=E=	Catalogue in electronic form as J/A+A/478/755
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CAX
CAX	(Chandra AE Aur X-ray source)
Write:	<<CAX NNN>>
N:	114
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS osbervations of N=114 X-ray sources in the field of AE Aur. See also [RMF2019].
Rem:	(a dash between the acronym and its contents is found in the literature)
Ref:	=2019ApJ...885..105R
by	RANGELOV B. , MONTMERLE T., FEDERMAN S.R., BOISSE P., GABICI S.
	Astrophys. J., 885, 105-105 (2019)
	Runaway O-star bow shocks as particle accelerators? The case of AE Aur revisited.
o	Table 2: <CAX NNN> (Nos 1-114). Fig. 7, Table 3: <[RMF2019] EVS-N> (Nos 1-5).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CAZ2013]
[CAZ2013]	(Chen+Arce+Zhang+, 2013)
Write:	<<[CAZ2013] PER 065 A>> <<[CAZ2013] NGC 1333 IRAS NAN>> <<[CAZ2013] IRAS 03282 MMSN>> <<[CAZ2013] IC 348 MMSN>> <<[CAZ2013] OMC3 MMS6 SMMN>> <<[CAZ2013] NGC 2024 FIR5 SMMN>> <<[CAZ2013] HH 212 MMS>> <<[CAZ2013] HH 212 MMSN>> <<[CAZ2013] HH 25 SMMN>> <<[CAZ2013] L723 VLA2 MMSN>>
Object:	(mm) + (smm) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	SMA1.3mm and 850µm observations of compact millimeter and/or submillimeter dust continuum emission in nearby clouds.
Ref:	=2013ApJ...768..110C
by	CHEN X. , ARCE H.G., ZHANG Q., BOURKE T.L., LAUNHARDT R., JORGENSEN J.K., LEE C.-F., FOSTER J.B., DUNHAM M.M., PINEDA J.E., HENNING T.
	Astrophys. J., 768, 110 (2013)
	SMA observations of class 0 protostars: a high angular resolution survey of protostellar binary systems.
o	Fig. 4, Table 4: <[CAZ2013] PER 065 A> (Nos A-C). Fig. 5, Table 5: <[CAZ2013] NGC 1333 IRAS NAN> (2A1-2A2, 4A1-4A2). Fig. 6, Table 5: <[CAZ2013] IRAS 03282 MMSN> (Nos MMS1-MMS2). Fig. 8, Table 4: <[CAZ2013] IC 348 MMSN> (Nos MMS1-MMS2). Fig. 11, Table 5: <[CAZ2013] OMC3 MMS6 SMMN> (Nos SMM1-SMM2), <[CAZ2013] NGC 2024 FIR5 SMMN> (Nos SMM1-SMM2). Fig. 12, Table 4: <[CAZ2013] HH 212 MMS> N=1. Fig. 12, Table 5: <[CAZ2013] HH 212 MMSN> (Nos MMS1-MMS3). Fig. 13, Table 5: <[CAZ2013] HH 25 SMMN> (Nos SMM1-SMM3). Fig. 17, Table 4: <[CAZ2013] L723 VLA2 MMSN> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CAZ2018]
[CAZ2018]	(Cibirka+Acebron+Zitrin+, 2018)
Write:	<<[CAZ2018] MACS JHHMM.m+DDMM N>> <<[CAZ2018] MACS JHHMM.m+DDMM N.N>> <<[CAZ2018] MACS JHHMM.m+DDMM cN.N>> <<[CAZ2018] Abell S295 N>> <<[CAZ2018] Abell S295 N.N>> <<[CAZ2018] Abell S295 c7.N>> <<[CAZ2018] Abell 697 N>> <<[CAZ2018] Abell 697 N.N>> <<[CAZ2018] Abell 697 p3.3>>
N:	6+6+3+22+18+9+12+2+1
Object:	Grav. lensed image + Poss. Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=22+18+9 gravitationally lensed images and N=12+2+1 gravitationally lensed image candidates of N=6+6+3 multiply-imaged background sources by four galaxy clusters. Use of data from the RELICS Hubble Treasury program. See also [AAZ2019], [ACZ2018], [CSA2018], [PSC2018].
in source:	MCS J0025.4-1222
in source:	MCS J0159.8-0849
in source:	ACO S 295
in source:	ACO 697
Ref:	=2018ApJ...863..145C
by	CIBIRKA N. , ACEBRON A., ZITRIN A., COE D., AGULLI I., ANDRADE-SANTOS F., BRADAC M., FRYE B., LIVERMORE R.C., MAHLER G., SALMON B., SHARON K., TRENTI M., UMETSU K., AVILA R., BRADLEY L., CARRASCO D., CERNY C., CZAKON N.G., DAWSON W.A., HOAG A.T., HUANG K.-H., JOHNSON T.L., JONES C., KIKUCHIHARA S., LAM D., LOVISARI L., MAINALI R., OESCH P.A., OGAZ S., OUCHI M., PAST M., PATERNO-MAHLER R., PETERSON A., RYAN R.E., SENDRA-SERVER I., STARK D.P., STRAIT V., TOFT S., VULCANI B.
	Astrophys. J., 863, 145-145 (2018)
	RELICS: strong lensing analysis of the galaxy clusters Abell S295, Abell 697, MACS J0025.4-1222 and MACS J0159.8-0849.
o	Figs 1-2, Tables 3-4: <[CAZ2018] MACS JHHMM.m+DDMM N> N=2+4, <[CAZ2018] MACS JHHMM.m+DDMM N.N> N=12+10, <[CAZ2018] MACS JHHMM.m+DDMM cN.N> N=8+4. Fig. 3, Table 5: <[CAZ2018] Abell S295 N> (Nos 1-6), <[CAZ2018] Abell S295 N.N> N=18 among (Nos 1.1-1.3 to 6.1-6.3), <[CAZ2018] Abell S295 c7.N> (Nos c7.1-c7.2). Fig. 4, Table 6: <[CAZ2018] Abell 697 N> (Nos 1-3), <[CAZ2018] Abell 697 N.N> N=9 among (Nos 1.1-1.4 to 3.1-3.2), <[CAZ2018] Abell 697 p3.3> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CB
CB	(C. Bertaud) (Not yet in Simbad)
*****	Avoid the usage of CB, prefer CB59
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CB
CB	(Clemens+Barvainis)
*****	Avoid the usage of CB, prefer [CB88]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CB
CB	(Cepa+Beckman)
*****	Avoid the usage of CB, prefer [CB90]
Origin	of the Acronym: L (1998A&A...331..601I)
Details on Acronym: Cb
Cb	(Cancer cl., bright)
*****	Avoid the usage of Cb, prefer [CSD91]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CB
CB	(Corona Borealis)
*****	Avoid the usage of CB, prefer [SSH97b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CB01
CB01	(Conti+Blum, 2001) (Not yet in Simbad)
Write:	<<CB01 W49 N>>
N:	9
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	N=9 new K-band sources. See also [DJW84].
in source:	W 49:W 49N = W 49N
Ref:	=2002ApJ...564..827C
by	CONTI P.S. , BLUM R.D.
	Astrophys. J., 564, 827-833 (2002)
	Near-infrared observations of the giant H II region W49A: a star birth cluster.
o	p. 829 : G29.96+0.6 misprint for G29.96-0.02
o	Figs 2, 3L <CB01 W 49 N> (Nos 1-9).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CB2003]
[CB2003]	(Carraro+Baume, 2003)
Write:	<<[CB2003] N-NNNN>>
N:	1460+2205+4486
Object:	* in Cl* (SIMBAD class: Star)
Note:	NTT EMMI photometry of the old clusters [SSW94] a, [SSW94] b, and [SSW94] c, objects 1-NNNN, 2-NNNN, 3-NNNN respectively. See also [FMP2006] for [SSW94] a.
in source:	[SSW94] a
in source:	[SSW94] b
in source:	[SSW94] c
Ref:	=2003MNRAS.346...18C
by	CARRARO G. , BAUME G.
	Mon. Not. R. Astron. Soc., 346, 18-26 (2003)
	The old open clusters Saurer A, B and C revisited.
o	Saurer A, B, C = respectively [SSW94] a, b, c
o	Saurer1.dat: <[CB2003] 1-NNNN> (Nos 1-1 to 1-1460). Saurer2.dat: <[CB2003] 2-NNNN> (Nos 2-1 to 2-2205). Saurer3.dat: <[CB2003] 3-NNNN> (Nos 3-1 to 3-4486).
=E=	Catalogue in electronic form as J/MNRAS/346/18
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CB2005]
[CB2005]	(Cellone+Buzzoni, 2005)
Write:	<<[CB2005] BN>>
N:	4
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ESO 3.6m telescope multicolour imaging of the NGC 5044 Group. N=4 background galaxies, not members of the NGC 5044 Group.
Ref:	=2005MNRAS.356...41C
by	CELLONE S.A. , BUZZONI A.
	Mon. Not. R. Astron. Soc., 356, 41-53 (2005)
	The low-luminosity galaxy population in the NGC5044 Group.
o	Table 2: <[CB2005] AN> (Nos B1-B4). Table 3: <[FS90] NGC 5044 NNNA> (Nos 54A, 64A, 70A, 93A-93C) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CB2009]
[CB2009]	(Crowther+Bibby, 2009)
Write:	<<[CB2009] A1-NW>> <<[CB2009] AN-WRN>> <<[CB2009] AN-HII N>> <<[CB2009] A1-C1>>
N:	1+7+4+1
Object:	Unknown (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT/FORS2 observations of giant HII regions within IC 4662. Use of archival HST/ACS data.
Ref:	=2009A&A...499..455C
by	CROWTHER P.A. , BIBBY J.L.
	Astron. Astrophys., 499, 455-464 (2009)
	On the massive star content of the nearby dwarf irregular Wolf-Rayet galaxy IC 4662.
o	Fig. 2, Table 4: <[CB2009] A1-NW>, <[CB2009] AN-WRN> (Nos A1-WR1 to A1-WR4, A2-WR1 to A2-WR3), <[CB2009] AN-HII N> (Nos A1-HII 1 to A1-HII 2, A2-HII 1 to A2-HII 2), <[CB2009] A1-C1>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CB2018]
[CB2018]	(Carretta+Bragaglia, 2018)
Write:	<<[CB2018] ANN>>
N:	17
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT UVES and ESO/MPG 2.2m telescope WFI observations of N=17 stars in NGC 6388. Use of 2MASS data.
in source:	NGC 6388
Ref:	=2018A&A...614A.109C
by	CARRETTA E. , BRAGAGLIA A.
	Astron. Astrophys., 614A, 109-109 (2018)
	Observing multiple populations in globular clusters with the ESO archive: NGC 6388 reloaded.
o	Table 1: <[CB2018] ANN> (Nos A01-A17).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CB2022]
[CB2022]	(Carretta+Bragaglia, 2022)
Write:	<<[CB2022] n63a>> <<[CB2022] l63pNNN>>
N:	12+150
Object:	* (SIMBAD class: Star)
Note:	VLT UVES and GIRAFFE spectroscopy of N=12+150 giant stars in the globular cluster NGC 6388.
in source:	NGC 6388
Ref:	=2022A&A...659A.122C
by	CARRETTA E. , BRAGAGLIA A.
	Astron. Astrophys., 659A, 122-122 (2022)
	Metallicity of the globular cluster NGC 6388 based on high-resolution spectra of more than 160 giant stars.
o	Tables 2-3: <[CB2022] n63a> N=12 among (Nos a-n), <[CB2022] l63pNNN> N=150 among (Nos 001-309).
=E=	Catalogue in electronic form as <J/A+A/659/A122/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: CB59
CB59	(C. Bertaud, 1959)= (CB) (Not yet in Simbad)
Write:	<<CB59 NNN>>
N:	476
Object:	A* (SIMBAD class: Star)
Note:	Superseded by Bertaud + Floquet, 1974A&AS...16...71B.
Ref:	=1959JO.....42...45B
by	BERTAUD C.
	J. Obs., 42, 45-None (1959)
	Catalogue et bibliographie des etoiles a spectre particulier.
o	Catalogue: <CB59 NNN> (Nos 1-476)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CB71]
[CB71]	(Ciatti+Barbon, 1971)
Write:	<<[CB71] NGC NNNN a>> <<[CB71] Anon HHMM+DDMM a>>
N:	4+9+5+7+7+8
Object:	* (SIMBAD class: Star)
Note:	Asiago systematic study of supernovae. Reference stars in the field of 6 galaxies host of SN
Ref:	=1971MmSAI..42..145C
by	CIATTI F. , BARBON R.
	Mem. Soc. Astron. Ital., 42, 145-161 (1971)
	Observations of six supernovae.
o	Fig.1: <[CB71] NGC 4753 a> (Nos a-d). Fig.4: <[CB71] NGC 3631 a> (Nos a-i). Fig.6: <[CB71] Anon 0912+4707 a> (Nos a-e). Fig.8: <[CB71] Anon 0434-0306 a> (Nos a-g). Fig.10: <[CB71] NGC 2713 a> (Nos a-g). Fig.12: <[CB71] NGC 3556 a> (Nos a-h).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CB85]
[CB85]	(Cowan+Branch, 1985)= (CRB)
Write:	<<[CB85] ggg>> <<[CB85] N>>
N:	6+8
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Format 'ggg' stands for greek letter (ex. alf) N=6 nonthermal sources. Format 'N', N=8 thermal sources.
in source:	M 83 = NGC 5236
Ref:	=1985ApJ...293..400C
by	COWAN J.J. , BRANCH D.
	Astrophys. J., 293, 400-406 (1985)
	Radio detection of historical supernovae and HII regions in M 83.
o	Table 1: <[CB85] aaa> N=5, "aaa" stands for greek letter. Table 2: <[CB85] N> N=8
Ref:	=1994ApJ...434..128C
by	COWAN J.J. , ROBERTS D.A., BRANCH D.
	Astrophys. J., 434, 128-135 (1994)
	Radio observations of M 83 and its supernova remnants.
o	<[CB85] zet> N=1 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CB88]
[CB88]	(Clemens+Barvainis, 1988)= (CB)
Write:	<<[CB88] NNN>> <<[CB88] NNN-N>>
N:	248+13
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-248) Molecular Clouds with an angular size less than 10' by selection associated IRAS detection. If 2 or more IRAS points within their boundaries, the format is 'NNN-N' for each source.. This format 'NNN-N' is coming from Launhardt Thesis (1996), and No. 58-2 appears first in 1996AJ....111..841Y. No Identif. charts See also YSO CBNNNYCN, YSO-C CBNNNYCN-R, [YMT96]
Ref:	=1988ApJS...68..257C
by	CLEMENS D.P. , BARVAINIS R.
	Astrophys. J., Suppl. Ser., 68, 257-286 (1988)
	A catalog of small, optically selected molecular clouds: optical, infrared, and millimeter properties.
o	cross-id Scho not in SIMBAD
o	<[CB88] NNN> (Nos 1-248)
Ref:	=1997A&A...326..329L
by	LAUNHARDT R. , HENNING T.
	Astron. Astrophys., 326, 329-346 (1997)
	Millimetre dust emission from northern Bok globules.
o	Table 1: <[CB88] NNN-N> N=13
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CB89]
[CB89]	(Carignan+Beaulieu, 1989)
Write:	<<[CB89] NN>>
N:	25
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	DDO 154
Ref:	=1989ApJ...347..760C
by	CARIGNAN C. , BEAULIEU S.
	Astrophys. J., 347, 760-770 (1989)
	Optical and HI studies of the "gas-rich" dwarf irregular galaxy DDO 154.
o	Table 5: <[CB89] NN> (Nos 1-25)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CB90]
[CB90]	(Cepa+Beckman, 1990)= (CB)
Write:	<<[CB90] NNN>>
N:	456
Object:	HII (SIMBAD class: HIIReg = HII Region)
in source:	NGC 4321
Ref:	=1990A&AS...83..211C
by	CEPA J. , BECKMAN J.E.
	Astron. Astrophys., Suppl. Ser., 83, 211-223 (1990)
	Distribution, sizes and luminosity function of the HII regions in NGC 4321.
o	Table I: <[CB90] NNN> (Nos 1-456)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CB95]
[CB95]	(Cox+Bronfman, 1995)
Write:	<<[CB95] AN>> <<[CB95] A>> <<[CB95] N>>
N:	4+8
Object:	Cloud (SIMBAD class: Cloud)
Note:	3 clouds A, B, and C, with cloud A divided into 2 subcomponents A1 and A2, and 8 clouds (Nos 1-8). See also [BBR2000].
in source:	NAME Keyhole Nebula
Ref:	=1995A&A...299..583C
by	COX P. , BRONFMAN L.
	Astron. Astrophys., 299, 583-590 (1995)
	The molecular gas content of the Keyhole nebula.
o	Fig. 1 and Table 1: <[CB95] AN> (Nos A1-A2), <[CB95] A> (Nos B-C), <[CB95] N> (Nos 1-5)
Ref:	=2002MNRAS.331....7S
by	SMITH N.
	Mon. Not. R. Astron. Soc., 331, 7-12 (2002)
	Near-infrared and optical emission-line structure of the Keyhole Nebula in NGC 3372.
o	Fig.2: <[CB95] N> (No. 6) added.
Ref:	=2002MNRAS.331...85R
by	RATHBORNE J.M. , BURTON M.G., BROOKS K.J., COHEN M., ASHLEY M.C.B., STOREY J.W.V.
	Mon. Not. R. Astron. Soc., 331, 85-97 (2002)
	Photodissociation regions and star formation in the Carina nebula.
o	p.93: sources 1, 3 = [MCB96] 1, 3.
o	Table 1, Fig.1: <[CB95] N> (Nos 7-8) added. Table 1, Fig.1: <[RBB2002] W> (Nos N, S). Table 4, Fig.11: <[RBB2002] WN> (Nos N1-N4), <[RBB2002] AN> (Nos R1-R3)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CB98]
[CB98]	(Cappa+Benaglia, 1998)
Write:	<<[CB98] LLL.l+B.b>>
N:	3
Object:	HI Bubble (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	N=3 HI bubbles associated with 3 stars HD 112244, 155913, 175754.
Ref:	=1998AJ....116.1906C
by	CAPPA C.E. , BENAGLIA P.
	Astron. J., 116, 1906-1914 (1998)
	The interstellar medium in the environs of O-type stars.
o	Table 2: <[CB98] LLL.l+B.b> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CB99]
[CB99]	(Codella+Bachiller, 1999)
Write:	<<[CB99] CB3-mm>> <<[CB99] Clump WN>>
N:	1+4
Object:	(mm) + Clump (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	IRAM 30m line observations of [CB99] 3. 'CB3-mm' designates the mm continuum source. N=4 features or clumps.
in source:	[CB88] 3
Ref:	=1999A&A...350..659C
by	CODELLA C. , BACHILLER R.
	Astron. Astrophys., 350, 659-671 (1999)
	Molecular outflows in intermediate-mass star forming regions: the case of CB3.
o	<[CB99] CB3-mm>. <[CB99] Clump WN> (Nos N1-N2, S1-S2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBA2002]
[CBA2002]	(Chary+Becklin+Armus, 2002) (Not yet in Simbad)
Write:	<<[CBA2002] GRB 991208 A>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Note:	Field of GRB 991208: 'A' is the host galaxy of the GRB, 'B' is a companion galaxy.
Ref:	=2002ApJ...566..229C
by	CHARY R. , BECKLIN E.E., ARMUS L.
	Astrophys. J., 566, 229-238 (2002)
	Are starburst galaxies the hosts of γ-ray bursts?
o	Fig.1: objects in GB 980613 = [HTN2002] A to E.
o	Fig.1: <[ZSB98] GN> (No. G4) added. Text: <[CBA2002] GRB 991208 A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBA2017]
[CBA2017]	(Carrasco+Barrientos+Anguita+, 2017) (Not yet in Simbad)
Write:	<<[CBA2017] SDSS JHHMM+DDMM SN.N>> <<[CBA2017] RCS2 JHHMM+DDMM SN.N>>
N:	53
Object:	Grav. lensed image of G (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy)
Note:	CFHT MegaCam, VLT FORS2, and Magellan 6.5m telescope IMACS observations of N=53 gravitaionally lensed images of galaxies in 29 strong lensing galaxy clusters.
Ref:	=2017ApJ...834..210C
by	CARRASCO M. , BARRIENTOS L.F., ANGUITA T., GARCIA-VERGARA C., BAYLISS M., GLADDERS M., GILBANK D., YEE H.K.C., WEST M.
	Astrophys. J., 834, 210-210 (2017)
	VLT/Magellan spectroscopy of 29 strong lensing selected galaxy clusters.
o	Table 2: <[CBA2017] SDSS JHHMM+DDMM SN.N> N=13, <[CBA2017] RCS2 JHHMM+DDMM SN.N> N=40.
=E=	Catalogue in electronic form as <J/ApJ/834/210/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBA94]
[CBA94]	(Cuisinier+Buser+Acker+, 1994)
Write:	<<[CBA94] NN>>
N:	49
Object:	PM* (SIMBAD class: HighPM* = High Proper Motion Star)
Stat:	is completely incorporated in Simbad
Ref:	=1994A&A...285..943C
by	CUISINIER F. , BUSER R., ACKER A., CAYREL R., JASNIEWICZ G., FRESNEAU A.
	Astron. Astrophys., 285, 943-952 (1994)
	Stellar atmospheric parameters for F-G-K stars from low-resolution data: method and application to a sample of proper motion stars.
o	<[CBA94] NN> N=49
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBA97]
[CBA97]	(Chrysostomou+Burton+Axon+, 1997)
Write:	<<[CBA97] NN>>
Object:	Bullet (SIMBAD class: PartofCloud = Part of Cloud)
Note:	UKIRT IRCAM Fabry-Perot observations. Discrete emission knots in the field of [RLK73] IRc 2 in OMC 1.
in source:	OMC:OMC 1 = OMC 1
Ref:	=1997MNRAS.289..605C
by	CHRYSOSTOMOU A. , BURTON M.G., AXON D.J., BRAND P.W.J.L., HOUGH J.H., BLAND-HAWTHORN J., GEBALLE T.R.
	Mon. Not. R. Astron. Soc., 289, 605-620 (1997)
	Velocity-resolved Fabry-Perot imaging of molecular hydrogen emission in OMC-1.
o	Table 4: <[CBA97] NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CBB
CBB	(CBB, CAMARGO+BONATTO+BICA)
Write:	<<CBB NN>>
N:	16
Object:	Poss. Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	Census of the star clusters towards the Galactic anticentre. Use of archival 2MASS data.
Ref:	=2011MNRAS.416.1522C
by	CAMARGO D. , BONATTO C., BICA E.
	Mon. Not. R. Astron. Soc., 416, 1522-1534 (2011)
	A possible sequential star formation in the giant molecular cloud G174+2.5.
o	Table 2: <CBB N> N=2 (Nos 1 and 2).
Ref:	=2012MNRAS.423.1940C
by	CAMARGO D. , BONATTO C., BICA E.
	Mon. Not. R. Astron. Soc., 423, 1940-1954 (2012)
	Towards a census of the Galactic anticentre star clusters – II. Exploring lower overdensities.
o	Table 3: <CBB N> N=7 (Nos 3-9) added.
Ref:	=2013MNRAS.432.3349C
by	CAMARGO D. , BICA E., BONATTO C.
	Mon. Not. R. Astron. Soc., 432, 3349-3360 (2013)
	Towards a census of the Galactic anticentre star clusters - III. Tracing the spiral structure in the outer disc.
o	Table 1: <CBB NN> N=7 (Nos 10-16) added.
=E=	Catalogue in electronic form as <J/MNRAS/432/3349/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CBB2001]
[CBB2001]	(Couch+Balogh+Bower+, 2001)= ([CBB2001a])
Write:	<<[CBB2001] NNNN>>
N:	586
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	HST observations of ACCG 114.
in source:	ACCG 114 = ACO S 1077
Ref:	=2001ApJ...549..820C
by	COUCH W.J. , BALOGH M.L., BOWER R.G., SMAIL I., GLAZEBROOK K., TAYLOR M.
	Astrophys. J., 549, 820-831 (2001)
	A low global star formation rate in the rich galaxy cluster AC 114 at z=0.32.
o	Table 1: <[CBB2001] NNNN> N=586 among (Nos 56-1629).
=E=	Catalogue in electronic form as J/ApJ/549/820
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBB2001a]
[CBB2001a]	(Couch+Balogh+Bower+, 2001)
*****	Avoid the usage of [CBB2001a], prefer [CBB2001]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBB2001b]
[CBB2001b]	(Cohen+Behr+Briley, 2001)
Write:	<<[CBB2001b] MMSS.s-MMSS>>
N:	14
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Keck observations. Coordinates 2000: RA = 19h, Dec = +18deg.
in source:	M 71 = NGC 6838
Ref:	=2001AJ....122.1420C
by	COHEN J.G. , BEHR B.B., BRILEY M.M.
	Astron. J., 122, 1420-1428 (2001)
	Abundances in stars from the red giant branch tip to near the main-sequence turnoff in M71. I. Sample selection, observing strategy, and stellar parameters.
o	Tables 1, 2: <[CBB2001b] MMSS.s-MMSS> N=14.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBB2003]
[CBB2003]	(Codella+Bachiller+Benedettini+, 2003) (Not yet in Simbad)
Write:	<<[CBB2003] A>>
N:	4
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Note:	N=4 high-velocity clumps in Cep A: Clumps A to C are H2S clumps, clump D is SO2 clump.
in source:	NAME Cep A
Ref:	=2003MNRAS.341..707C
by	CODELLA C. , BACHILLER R., BENEDETTINI M., CASELLI P.
	Mon. Not. R. Astron. Soc., 341, 707-716 (2003)
	Shocked gas around Cepheus A: evidence for multiple outflows from H_{2}S and SO_{2}observations.
o	Fig.1: <[CBB2003] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBB2004]
[CBB2004]	(Cross+Bouwens+Benitez+, 2004)
Write:	<<[CBB2004] NN>>
N:	72
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations. Measurement of the luminosity function of morphologically selected E/S0 galaxies with redshift from 0.5 to 1.5 in 5 fields.
Ref:	=2004AJ....128.1990C
by	CROSS N.J.G. , BOUWENS R.J., BENITEZ N., BLAKESLEE J.P., MENANTEAU F., FORD H.C., GOTO T., HOLDEN B., MARTEL A.R., ZIRM A., OVERZIER R., GRONWALL C., HOMEIER N., CLAMPIN M., HARTIG G.F., ILLINGWORTH G.D., ARDILA D.R., BARTKO F., BROADHURST T.J., BROWN R.A., BURROWS C.J., CHENG E.S., FELDMAN P.D., FRANX M., GOLIMOWSKI D.A., INFANTE L., KIMBLE R.A., KRIST J.E., LESSER M.P., MEURER G.R., MILEY G.K., POSTMAN M., ROSATI P., SIRIANNI M., SPARKS W.B., TRAN H.D., TSVETANOV Z.I., WHITE R.L., ZHENG W.
	Astron. J., 128, 1990-2012 (2004)
	The luminosity function of early-type field galaxies at z~0.75.
o	Table 2: <[CBB2004] NN> (Nos 1-72).
=E=	Catalogue in electronic form as J/AJ/128/1990
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBB2008]
[CBB2008]	(Cooke+Barton+Bullock+, 2008) (Not yet in Simbad)
Write:	<<[CBB2008] A>>
N:	5
Object:	Component (SIMBAD class: PartofG = Part of a Galaxy)
Note:	LRIS Spectroscopy of LBG-2377.
in source:	NAME LBG-2377
Ref:	=2008ApJ...681L..57C
by	COOKE J. , BARTON E.J., BULLOCK J.S., STEWART K.R., WOLFE A.M.
	Astrophys. J., 681L, 57-60 (2008)
	A candidate brightest protocluster galaxy at z = 3.03.
o	Table 1: <[CBB2008] A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBB2009]
[CBB2009]	(Cantiello+Brocato+Blakeslee, 2009)
Write:	<<[CBB2009] NNN>>
N:	277
Object:	Poss. Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST ACS observations of star clusters in NGC 3370.
in source:	NGC 3370
Ref:	=2009A&A...503...87C
by	CANTIELLO M. , BROCATO E., BLAKESLEE J.P.
	Astron. Astrophys., 503, 87-101 (2009)
	The star cluster population of the spiral galaxy NGC 3370.
o	Table 3: <[CBB2009] NNN> N=277 among (Nos 5-633).
=E=	Catalogue in electronic form as J/A+A/503/87
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBB2010]
[CBB2010]	(Cooke+Berrier+Barton+, 2011)= ([CBB2010a])
Write:	<<[CBB2010] Pair HHMM-NNNN>>
N:	5
Object:	Pair of G (SIMBAD class: PairG = Pair of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Keck I LRIS observations of N=5 serendipitous spectroscopic close pairs of galaxies.
Ref:	=2010MNRAS.403.1020C
by	COOKE J. , BERRIER J.C., BARTON E.J., BULLOCK J.S., WOLFE A.M.
	Mon. Not. R. Astron. Soc., 403, 1020-1035 (2010)
	Lyman break galaxy close and interacting pairs at z ~ 3.
o	In Chap. 6 and Fig. 8: Objects LAE and LBG are not identified.
o	Table 1: <[CBB2010] Pair HHMM-NNNN> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBB2010a]
[CBB2010a]	(Cooke+Berrier+Barton+, 2011) (Not yet in Simbad)
*****	Avoid the usage of [CBB2010a], prefer [CBB2010]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBB2010b]
[CBB2010b]	(Coe+Benitez+Broadhurst+, 2010)
Write:	<<[CBB2010b] A1689 NNN>> <<[CBB2010b] NNa>> <<[CBB2010b] NNa N>> <<[CBB2010b] NN>>
N:	113+135+33+42
Object:	* + G + Grav. lensed image of a G + Part of G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST ACS observations of the galaxy cluster ACO 1689. Format A1689 NNN: N=113 sources in the field of view. Format NN: N=42 galaxies gravitationally lensed by ACO 1689. Format NNa: N=135 images of the 42 lensed galaxies. Format NNa N: N=33 knots in 8 of the 42 lensed galaxies.
in source:	ACO 1689
Ref:	=2010ApJ...723.1678C
by	COE D. , BENITEZ N., BROADHURST T., MOUSTAKAS L.A.
	Astrophys. J., 723, 1678-1702 (2010)
	A high-resolution mass map of galaxy cluster substructure: LensPerfect analysis of A1689.
o	Table 4: <[CBB2010b] A1689 NNN> N=113 among (Nos 1-452). Table 5: <[CBB2010b] NNa> N=135 among (Nos 1a-1f to 50a-50c). Table 6: <[CBB2010b] NNa N> N=33. Table 7: <[CBB2010b] NN> N=42 among (Nos 1-50).
=E=	Catalogue in electronic form as J/ApJ/723/1678
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBB2012]
[CBB2012]	(Casey+Berta+Bethermin+, 2012)= (1HERMES)
Write:	<<[CBB2012] {1HERMES} {X1.4\|X24} JHHMMSS.ss+DDMMSS.s>>
N:	326+441
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck I LRIS and Keck II DEIMOS observations of N=731+36 Herschel-SPIRE selected galaxies at z<2. Counterpart identification and point source photometry are performed at known positions of Spitzer-MIPS 24µm and Very Large Array 1.4GHz sources. Hence the X1.4 or X24 in format. 2012ApJ...761..139C: N=36 galaxies at 2<z<5. 2012ApJ...761..140C: N=731 galaxies at z<2.
Ref:	=2012ApJ...761..140C
by	CASEY C.M. , BERTA S., BETHERMIN M., BOCK J., BRIDGE C., BUDYNKIEWICZ J., BURGARELLA D., CHAPIN E., CHAPMAN S.C., CLEMENTS D.L., CONLEY A., CONSELICE C.J., COORAY A., FARRAH D., HATZIMINAOGLOU E., IVISON R.J., LE FLOC'H E., LUTZ D., MAGDIS G., MAGNELLI B., OLIVER S.J., PAGE M.J., POZZI F., RIGOPOULOU D., RIGUCCINI L., ROSEBOOM I.G., SANDERS D.B., SCOTT D., SEYMOUR N., VALTCHANOV I., VIEIRA J.D., VIERO M., WARDLOW J.
	Astrophys. J., 761, 140 (2012)
	A redshift survey of Herschel far-infrared selected starbursts and implications for obscured star formation.
o	Table 1: <[CBB2012] 1HERMES X1.4 JHHMMSS.ss+DDMMSS.s> N=302, <[CBB2012] 1HERMES X24 JHHMMSS.ss+DDMMSS.s> N=418.
Ref:	=2012ApJ...761..139C
by	CASEY C.M. , BERTA S., BETHERMIN M., BOCK J., BRIDGE C., BURGARELLA D., CHAPIN E., CHAPMAN S.C., CLEMENTS D.L., CONLEY A., CONSELICE C.J., COORAY A., FARRAH D., HATZIMINAOGLOU E., IVISON R.J., FLOC'H E.L., LUTZ D., MAGDIS G., MAGNELLI B., OLIVER S.J., PAGE M.J., POZZI F., RIGOPOULOU D., RIGUCCINI L., ROSEBOOM I.G., SANDERS D.B., SCOTT D., SEYMOUR N., VALTCHANOV I., VIEIRA J.D., VIERO M., WARDLOW J.
	Astrophys. J., 761, 139 (2012)
	A population of z > 2 far-infrared Herschel-SPIRE-selected starbursts.
o	Table 1: <[CBB2012] 1HERMES X1.4 JHHMMSS.ss+DDMMSS.s> N=16, <[CBB2012] 1HERMES X24 JHHMMSS.ss+DDMMSS.s> N=20.
=E=	Catalogue in electronic form as J/ApJ/761/140
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBB2013]
[CBB2013]	(Chene+Borissova+Bonatto+, 2013)= ([CBB2013a])
Write:	<<[CBB2013] VVV CLNNN NN>>
N:	91
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	NTT SofI, SOAR OSIRIS and VLT ISAAC NIR spectroscopy of N=51 stars in six young, massive open clusters. Use of data from the ESO Public Survey "VISTA Variables in the Via Lactea" (VVV). 2019A&A...627A.170M: VLT SINFONI observations of N=40 additional stars in VVV CL074.
in source:	VVV CL009
in source:	VVV CL011
in source:	VVV CL036
in source:	VVV CL073
in source:	VVV CL074
in source:	VVV CL099
Ref:	=2013A&A...549A..98C
by	CHENE A.-N. , BORISSOVA J., BONATTO C., MAJAESS D.J., BAUME G., CLARKE J.R.A., KURTEV R., SCHNURR O., BOURET J.-C., CATELAN M., EMERSON J.P., FEINSTEIN C., GEISLER D., DE GRIJS R., HERVE A., IVANOV V.D., KUMAR M.S.N., LUCAS P., MAHY L., MARTINS F., MAURO F., MINNITI D., MONI BIDIN C.
	Astron. Astrophys., 549A, 98-98 (2013)
	Massive open star clusters using the VVV survey. II. Discovery of six clusters with Wolf-Rayet stars.
o	Table 3: <[CBB2013] VVV CLNNN NN> N=51.
Ref:	=2019A&A...627A.170M
by	MARTINS F. , CHENE A.-N., BOURET J.-C., BORISSOVA J., GROH J., RAMIREZ ALEGRIA S., MINNITI D.
	Astron. Astrophys., 627A, 170-170 (2019)
	Massive stars in the young cluster VVV CL074.
o	Table 1: <[CBB2013] VVV CL074 NN> (Nos 12-51) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBB2013a]
[CBB2013a]	(Chene+Borissova+Bonatto+, 2013)
*****	Avoid the usage of [CBB2013a], prefer [CBB2013]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBB2013b]
[CBB2013b]	(Carraro+Buzzoni+Bertone+, 2013)
Write:	<<[CBB2013b] NNNN>>
N:	15
Object:	* (SIMBAD class: Star)
Note:	TNG DOLORES observations of N=15 stars in the field of NGC 6791.
in source:	NGC 6791
Ref:	=2013AJ....146..128C
by	CARRARO G. , BUZZONI A., BERTONE E., BUSON L.
	Astron. J., 146, 128 (2013)
	UB CCD photometry of the old, metal-rich, open clusters NGC 6791, NGC 6819, and NGC 7142.
o	Table 1, PG2213+006 is a probable misprint for PG2213-006.
o	Tables 4-5: <[CBB2013b] NNNN> N=15 among (Nos 156-7068).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBB2014]
[CBB2014]	(Calchi Novati+Bozza+Bruni, 2014) (Not yet in Simbad)
Write:	<<[CBB2014] OAB-10-S3>>
N:	1
Object:	Poss. Microlensing Event (SIMBAD class: LensingEv = (Micro)Lensing Event)
Note:	Loiano 152cm Cassini telescope observations of N=1 microlensing candidate toward M31. See also [CBD2009].
Ref:	=2014ApJ...783...86C
by	CALCHI NOVATI S. , BOZZA V., BRUNI I., DALL'ORA M., DE PAOLIS F., DOMINIK M., GUALANDI R., INGROSSO G., JETZER Ph., MANCINI L., NUCITA A., SAFONOVA M., SCARPETTA G., SERENO M., STRAFELLA F., SUBRAMANIAM A., GOULD A., (The PLAN Collaboration)
	Astrophys. J., 783, 86 (2014)
	The M31 pixel lensing PLAN campaign: MACHO lensing and self-lensing signals.
o	Fig. 1: <[CBB2014] OAB-10-S3> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBB2017]
[CBB2017]	(Corbelli+Braine+Bandiera+, 2017)
Write:	<<[CBB2017] NNN>>
N:	566
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	IRAM 30m telescope CO(2-1) observations of N=566 giant molecular clouds (GMCs) in M 33 disk. See also [VHC2017b].
in source:	M 33 = NGC 598
Ref:	=2017A&A...601A.146C
by	CORBELLI E. , BRAINE J., BANDIERA R., BROUILLET N., COMBES F., DRUARD C., GRATIER P., MATA J., SCHUSTER K., XILOURIS M., PALLA F.
	Astron. Astrophys., 601A, 146-146 (2017)
	From molecules to young stellar clusters: the star formation cycle across the disk of M 33.
o	Table 5: <[CBB2017] NNN> (Nos 1-566).
=E=	Catalogue in electronic form as J/A+A/601/A146
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBB98]
[CBB98]	(Cabanac+Borra+Beauchemin, 1998)
Write:	<<[CBB98] NNN>>
N:	206
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	NASA Orbital Debris Observatory astronomical survey
Ref:	=1998ApJ...509..309C
by	CABANAC R.A. , BORRA E.F., BEAUCHEMIN M.
	Astrophys. J., 509, 309-323 (1998)
	A search for peculiar objects with the NASA orbital debris observatory 3 meter liquid mirror telescope.
o	Table 3: <[CBB98] NNN> (Nos 1-206).
=E=	Catalogue in electronic form as J/ApJ/509/309
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBC2005]
[CBC2005]	(Costado+Bejar+Caballero+, 2005)
Write:	<<[CBC2005] N>>
N:	4
Object:	Brown Dwarf (SIMBAD class: BrownD* = Brown Dwarf)
Note:	TNG and WHT observations. Search for faint companions to [PBB2002] USco stars from UScoCTIO and [PBB2002]: none is detected. 4 ultracool isolated objects are found near 4 [PBB2002] USco stars.
in source:	NAME Upper Sco Assoc
Ref:	=2005A&A...443.1021C
by	COSTADO M.T. , BEJAR V.J.S., CABALLERO J.A., REBOLO R., ACOSTA-PULIDO J., MANCHADO A.
	Astron. Astrophys., 443, 1021-1024 (2005)
	A search for planetary-mass objects and brown dwarfs in the Upper Scorpius association.
o	Table 3: <[CBC2005] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBC2007]
[CBC2007]	(Coble+Bonamente+Carlstrom+, 2007)= ([CBC2007a])
Write:	<<[CBC2007] JHHMMSS.s+DDMMSS.s>>
N:	117+4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	BIMA and OVRO arrays deep interferometric observations at 28.8 GHz. Sources in 89 galaxy clusters and 4 noncluster fields.
Ref:	=2007AJ....134..897C
by	COBLE K. , BONAMENTE M., CARLSTROM J.E., DAWSON K., HASLER N., HOLZAPFEL W., JOY M., LAROQUE S., MARRONE D.P., REESE E.D.
	Astron. J., 134, 897-905 (2007)
	Radio sources toward galaxy clusters at 30 GHz.
o	Table 1, col(11,12), Table 2, col(5,6): <[CBC2007] JHHMMSS.s+DDMMSS.s> N=117+4.
=E=	Catalogue in electronic form as J/AJ/134/897
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBC2007a]
[CBC2007a]	(Coble+Bonamente+Carlstrom+, 2007)
*****	Avoid the usage of [CBC2007a], prefer [CBC2007]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBC2007b]
[CBC2007b]	(Chary+Berger+Cowie, 2007)
Write:	<<[CBC2007b] GRB 060510B Host G>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spitzer observations of the host galaxy of GRB 060510B.
Ref:	=2007ApJ...671..272C
by	CHARY R. , BERGER E., COWIE L.
	Astrophys. J., 671, 272-277 (2007)
	Spitzer observations of γ-ray burst host galaxies: a unique window into high-redshift chemical evolution and star formation.
o	<[CBC2007b] GRB 060510B Host G> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBC2012]
[CBC2012]	(Chene+Borissova+Clarke+, 2012)
Write:	<<[CBC2012] ObjNN>> <<[CBC2012] DN-NNNN>> <<[CBC2012] RCW79-NNNN>>
N:	45+89+36
Object:	* + V* (SIMBAD class: Star)
Note:	Use of data from the ESO Public Survey "VISTA Variables in the Via Lactea" (VVV) and complementary low-resolution NIR spectroscopy (NTT and Las Campanas Clay telescope) of known massive star clusters.
in source:	Cl Danks 1
in source:	Cl Danks 2
in source:	RCW 79
in source:	[DBS2003] 132
Ref:	=2012A&A...545A..54C
by	CHENE A.-N. , BORISSOVA J., CLARKE J.R.A., BONATTO C., MAJAESS D.J., MONI BIDIN C., SALE S.E., MAURO F., KURTEV R., BAUME G., FEINSTEIN C., IVANOV V.D., GEISLER D., CATELAN M., MINNITI D., LUCAS P., DE GRIJS R., KUMAR M.S.N.
	Astron. Astrophys., 545A, 54-54 (2012)
	Massive open star clusters using the VVV survey. I. Presentation of the data and description of the approach.
o	Table 2: <[CBC2012] ObjNN> (Nos 1-45). Table 5: <[CBC2012] DN-NNNN> N=60+29 among (Nos D1-0078 to D1-3544, D2-0007 to D2-3203). Table 6: <[CBC2012] RCW79-NNNN> N=36 among (Nos 0029-1399).
=E=	Catalogue in electronic form as <J/A+A/545/A54/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBC2016]
[CBC2016]	(Chavez-Dagostino+Bertone+Cruz-Saenz De Miera+, 2016)
Write:	<<[CBC2016] SN>>
N:	7
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	LMT AzTEC 1.1m continuum observations of N=7 background millimeter sources in the field of ε Eridani.
in source:	* eps Eri
Ref:	=2016MNRAS.462.2285C
by	CHAVEZ-DAGOSTINO M. , BERTONE E., CRUZ-SAENZ DE MIERA F., MARSHALL J.P., WILSON G.W., SANCHEZ-ARGUELLES D., HUGHES D.H., KENNEDY G., VEGA O., DE LA LUZ V., DENT W.R.F., EIROA C., GOMEZ-RUIZ A.I., GREAVES J.S., LIZANO S., LOPEZ-VALDIVIA R., MAMAJEK E., MONTANA A., OLMEDO M., RODRIGUEZ-MONTOYA I., SCHLOERB F.P., YUN M.S., ZAVALA J.A., ZEBALLOS M.
	Mon. Not. R. Astron. Soc., 462, 2285-2294 (2016)
	Early science with the Large Millimetre Telescope: Deep LMT/AzTEC millimetre observations of ε Eridani and its surroundings.
o	Fig. 1, Table 1: <[CBC2016] SN> (Nos S1-S7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBD2002]
[CBD2002]	(Cotter+Buttery+Das+, 2002)
Write:	<<[CBD2002] JHHMMSS.sss+DDMMSS.ss>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Ryle Telescope observations. N=4 radio-sources in the field of 1E 1137.5+6625.
Ref:	=2002MNRAS.334..323C
by	COTTER G. , BUTTERY H.J., DAS R., JONES M.E., GRAINGE K., POOLEY G.G., SAUNDERS R.
	Mon. Not. R. Astron. Soc., 334, 323-326 (2002)
	Observations of the Sunyaev-Zel'dovich effect in the z =0.78 cluster MS 1137.5+6625.
o	Table 1: <[CBD2002] JHHMMSS.sss+DDMMSS.ss> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBD2003]
[CBD2003]	(Cappi+Benoist+Da Costa+, 2003)
Write:	<<[CBD2003] VLG NNN NNN>> <<[CBD2003] VLG 0716+5323 N>>
N:	802+9
Object:	G (SIMBAD class: Galaxy)
Note:	OHP observations and 2dFGRS 100k data of environment of VLG (Very Luminous G). See also [CDB98].
Ref:	=2003A&A...408..905C
by	CAPPI A. , BENOIST C., DA COSTA L.N., MAUROGORDATO S.
	Astron. Astrophys., 408, 905-913 (2003)
	Nature and environment of Very Luminous Galaxies.
o	Table 1 : VLG 0716+5323 field = LEDA 20561 field, Z1261 = RXC J0716.7+5324.
o	Tables 1, B1-B15: <[CBD2003] VLG NNN NNN> N=802, <[CBD2003] VLG 0716+5323 N> (Nos 1-9).
=E=	Catalogue in electronic form as J/A+A/408/905
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBD2009]
[CBD2009]	(Calchi Novati+Bozza+De Paolis+, 2009)
Write:	<<[CBD2009] OAB-NN>>
N:	2
Object:	Microlensing Event (SIMBAD class: LensingEv = (Micro)Lensing Event)
Stat:	is completely incorporated in Simbad
Note:	Loiano 152cm Cassini telescope observations of N=2 candidate microlensing events toward M31.
Ref:	=2009ApJ...695..442C
by	CALCHI NOVATI S. , BOZZA V., DE PAOLIS F., DOMINIK M., INGROSSO G., JETZER P., MANCINI L., NUCITA A., SCARPETTA G., SERENO M., STRAFELLA F., GOULD A.
	Astrophys. J., 695, 442-454 (2009)
	Candidate microlensing events from M31 observations with the Loiano telescope.
o	Table 3: <[CBD2009] OAB-NN> (Nos OAB-N1 to OAB-N2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBD2011]
[CBD2011]	(Cappa+Barba+Duronea+, 2017) (Not yet in Simbad)
Write:	<<[CBD2011] GLLL.ll+BB.bb>>
N:	3
Object:	Region (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	CTIO Curtis-Schmidt (optical), VLA (20cm) and NANTEN (CO) observations of N=3 structures in NGC 6357.
in source:	NGC 6357
Ref:	=2011MNRAS.415.2844C
by	CAPPA C.E. , BARBA R., DURONEA N.U., VASQUEZ J., ARNAL E.M., GOSS W.M., FERNANDEZ LAJUS E.
	Mon. Not. R. Astron. Soc., 415, 2844-2858 (2011)
	A multifrequency study of the active star-forming complex NGC 6357 – I. Interstellar structures linked to the open cluster Pis 24.
o	Figs 2+5, Table 1: <[CBD2011] GLLL.ll+BB.bb> (Nos G353.12+00.86, G353.19+00.84, G353.24+00.64).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CBF
CBF	(Chandar+Bianchi+Ford)= (CBF01)
Write:	<<CBF NNN>> <<CBF AA N-N>>
N:	162
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of M 33. N=162 star clusters in M 33, (Nos 1-162). In the 1st paper, the clusters have a 2nd format 'AA N-N' where 'AA N' stands for WFPC2 fields.
in source:	M 33 = NGC 598
Ref:	=1999ApJS..122..431C
by	CHANDAR R. , BIANCHI L., FORD H.C.
	Astrophys. J., Suppl. Ser., 122, 431-464 (1999)
	Star clusters in M33. I. Detection, morphology, and photometry.
o	Table 2: <CBF AA N-N> = <CBF NN> (Nos 1-60).
Ref:	=2001A&A...366..498C
by	CHANDAR R. , BIANCHI L., FORD H.C.
	Astron. Astrophys., 366, 498-507 (2001)
	Star clusters in M 33. IV. A new survey from deep HST images.
o	in ref list Holtzman et al 1995PASP.107.1065 instead of 106
o	Table 2: <CBF NNN> (Nos 61-162) added.
=E=	Catalogue in electronic form as J/ApJS/122/431
Origin	of the Acronym: L (1999PASP..111..794C)
Details on Acronym: CBF
CBF	(Chandar+Bianchi+Ford+)
*****	Avoid the usage of CBF, prefer [CBF2002]
Origin	of the Acronym: L (2007AJ....134..447S)
Details on Acronym: CBF01
CBF01	(Chandar+Bianchi+Ford, 2001)
*****	Avoid the usage of CBF01, prefer CBF
Origin	of the Acronym: L (2007AJ....133..290S)
Details on Acronym: [CBF2002]
[CBF2002]	(Chandar+Bianchi+Ford+, 2002)= (CBF) = ([CBF2002a])
Write:	<<[CBF2002] NNN>>
N:	111
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	WIYN HYDRA spectroscopy of star clusters in M33.
in source:	M 33 = NGC 598
Ref:	=2002ApJ...564..712C
by	CHANDAR R. , BIANCHI L., FORD H.C., SARAJEDINI A.
	Astrophys. J., 564, 712-735 (2002)
	Kinematics of star clusters in M33: distinct populations.
o	p. 718 : Star clusters 158 and 225 in M31 = SKHB ??
o	Table 1: <[CBF2002] NNN> (Nos 1-111).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBF2002a]
[CBF2002a]	(Chandar+Bianchi+Ford+, 2002)
*****	Avoid the usage of [CBF2002a], prefer [CBF2002]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBF2002b]
[CBF2002b]	(Catelan+Borissova+Ferraro+, 2002) (Not yet in Simbad)
Write:	<<[CBF2002b] xxxx.xxx-yyyy.yyy>>
N:	26
Object:	* in Cluster (SIMBAD class: Star)
in source:	M 75 = NGC 6864
Ref:	=2002AJ....124..364C
by	CATELAN M. , BORISSOVA J., FERRARO F.R., CORWIN T.M., SMITH H.A., KURTEV R.
	Astron. J., 124, 364-378 (2002)
	M75, a globular cluster with a trimodal horizontal branch. I. Color-magnitude diagram.
o	Table 5: <[CBF2002b] xxxx.xxx-yyyy.yyy> N=26.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBF2011]
[CBF2011]	(Capitanio+Bird+Fiocchi+, 2011) (Not yet in Simbad)
Write:	<<[CBF2011] WFC JHHMM+DDMM>>
N:	10+1
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Use of BeppoSAX WFC data. See also SAXWFC.
Ref:	=2011ApJS..195....9C
by	CAPITANIO F. , BIRD A.J., FIOCCHI M., SCARINGI S., UBERTINI P.
	Astrophys. J., Suppl. Ser., 195, 9 (2011)
	Finding persistent sources with the BeppoSAX/Wide Field Camera: an in-depth analysis.
o	In table 3, AXS J053514-0523 = SAXWFC J0535.3-0525.4 in Simbad.
o	Tables 3-4: <[CBF2011] WFC JHHMM+DDMM> N=11.
=E=	Catalogue in electronic form as <J/ApJS/195/9/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBF86]
[CBF86]	(Clarke+Burns+Feigelson, 1986)
Write:	<<[CBF86] SN>> <<[CBF86] WAN>>
N:	4+4+4
Object:	Feature (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=4 apparent filaments or Streamers in the radio jet of Cen A. N=4 Northern Lobe features (Nos NL1 to NL4) and N=4 Southern Lobe features (Nos SL1 to SL4). See also BGLO.
in source:	Cen A = NGC 5128
Ref:	=1986ApJ...300L..41C
by	CLARKE D.A. , BURNS J.O., FEIGELSON E.D.
	Astrophys. J., 300, 41-46 (1986)
	Limb brightening and filamentation in the inner radio jet of Centaurus A.
o	Knots are BGLO objects in SIMBAD, Streamers are [CBF86] SN.
o	Table 1, Fig.1: <BGLO Cen A Knot A1a> (Nos A1a-A1c), <[CBF86] SN> (Nos S1-S4).
Ref:	=1992ApJ...395..444C
by	CLARKE D.A. , BURNS J.O., NORMAN M.L.
	Astrophys. J., 395, 444-452 (1992)
	VLA observations of the inner lobes of Centaurus A.
o	Streamers S1 to S4 = [CBF86] S1 to S4.
o	Table 3, Fig.1: <[CBF86] WAN> (Nos NL1 to NL4, SL1 to SL4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBG2009]
[CBG2009]	(Carretta+Bragaglia+Gratton+, 2009)
Write:	<<[CBG2009] NGC NNNN NNNNNNN>>
N:	1529+202
Object:	RGB* (SIMBAD class: RGB* = Red Giant Branch star)
Stat:	is completely incorporated in Simbad
Note:	ESO FLAMES+GIRAFFE observations of 15+17 globular clusters.
Ref:	=2009A&A...505..117C
by	CARRETTA E. , BRAGAGLIA A., GRATTON R.G., LUCATELLO S., CATANZARO G., LEONE F., BELLAZZINI M., CLAUDI R., D'ORAZI V., MOMANY Y., ORTOLANI S., PANCINO E., PIOTTO G., RECIO-BLANCO A., SABBI E.
	Astron. Astrophys., 505, 117-138 (2009)
	Na-O anticorrelation and HB. VII. The chemical composition of first and second-generation stars in 15 globular clusters from GIRAFFE spectra.
o	Tables 2-3, 6: <[CBG2009] NGC NNNN NNNNNNN> N=1529.
Ref:	=2009A&A...505..139C
by	CARRETTA E. , BRAGAGLIA A., GRATTON R., LUCATELLO S.
	Astron. Astrophys., 505, 139-155 (2009)
	Na-O anticorrelation and HB. VIII. Proton-capture elements and metallicities in 17 globular clusters from UVES spectra.
o	Tables 3-4, 9: <[CBG2009] NGC NNNN NNNNNNN> N=202.
=E=	Catalogue in electronic form as J/A+A/505/117
=E=	Catalogue in electronic form as J/A+A/505/139
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBG2010]
[CBG2010]	(Carretta+Bragaglia+Gratton+, 2010)
Write:	<<[CBG2010] NNNNNNNN>>
N:	103
Object:	RGB* (SIMBAD class: RGB* = Red Giant Branch star)
Note:	VLT FLAMES observations of N=76+27 red giant stars in M54 and the nucleus of the Sagittarius dwarf galaxy, respectively.
in source:	M 54 = NGC 6715
in source:	NAME SDG = NAME Sgr Dwarf Galaxy
Ref:	=2010A&A...520A..95C
by	CARRETTA E. , BRAGAGLIA A., GRATTON R.G., LUCATELLO S., BELLAZZINI M., CATANZARO G., LEONE F., MOMANY Y., PIOTTO G., D'ORAZI V.
	Astron. Astrophys., 520A, 95-95 (2010)
	Detailed abundances of a large sample of giant stars in M 54 and in the Sagittarius nucleus.
o	Tables 2-3, 5-7: <[CBG2010] NNNNNNNN> N=103 among (Nos 15001387-42146527).
=E=	Catalogue in electronic form as J/A+A/520/A95
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBG2014]
[CBG2014]	(Carretta+Bragaglia+Gratton+, 2014)
Write:	<<[CBG2014] NNNNN>>
N:	78
Object:	RGB* (SIMBAD class: RGB* = Red Giant Branch star)
Note:	VLT FLAMES (GIRAFFE and UVES) observations of N=78 red giant members of the globular cluster NGC 4833.
in source:	NGC 4833
Ref:	=2014A&A...564A..60C
by	CARRETTA E. , BRAGAGLIA A., GRATTON R.G., D'ORAZI V., LUCATELLO S., MOMANY Y., SOLLIMA A., BELLAZZINI M., CATANZARO G., LEONE F.
	Astron. Astrophys., 564A, 60-60 (2014)
	The extreme chemistry of multiple stellar populations in the metal-poor globular cluster NGC 4833.
o	Table 2: <[CBG2014] NNNNN> N=78 among (Nos 22810-38029).
=E=	Catalogue in electronic form as J/A+A/564/A60
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBG2015]
[CBG2015]	(Carretta+Bragaglia+Gratton+, 2015)
Write:	<<[CBG2015] NNNNN>>
N:	143
Object:	Red * (SIMBAD class: RGB* = Red Giant Branch star)
Note:	ESO 2.2m WFI photometry and VLT FLAMES/GIRAFFE-UVES spectroscopy of N=143 red giant branch stars in the globular cluster NGC 6093.
in source:	NGC 6093 = M 80
Ref:	=2015A&A...578A.116C
by	CARRETTA E. , BRAGAGLIA A., GRATTON R.G., D'ORAZI V., LUCATELLO S., SOLLIMA A., MOMANY Y., CATANZARO G., LEONE F.
	Astron. Astrophys., 578A, 116-116 (2015)
	The normal chemistry of multiple stellar populations in the dense globular cluster NGC 6093 (M 80).
o	Tables 2-3,5-9: <[CBG2015] NNNNN> N=143 among (Nos 208-22172).
=E=	Catalogue in electronic form as J/A+A/578/A116
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBG2016]
[CBG2016]	(Connaughton+Burns+Goldstein+, 2016)
Write:	<<[CBG2016] GW150914-GBM>>
N:	1
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Fermi Gamma-ray Burst Monitor (GBM) observations of N=1 possible electromagnetic counterpart to the gravitational wave event GW150914.
Ref:	=2016ApJ...826L...6C
by	CONNAUGHTON V. , BURNS E., GOLDSTEIN A., BLACKBURN L., BRIGGS M.S., ZHANG B.-B., CAMP J., CHRISTENSEN N., HUI C.M., JENKE P., LITTENBERG T., McENERY J.E., RACUSIN J., SHAWHAN P., SINGER L., VEITCH J., WILSON-HODGE C.A., BHAT P.N., BISSALDI E., CLEVELAND W., FITZPATRICK G., GILES M.M., GIBBY M.H., VON KIENLIN A., KIPPEN R.M., McBREEN S., MAILYAN B., MEEGAN C.A., PACIESAS W.S., PREECE R.D., ROBERTS O.J., SPARKE L., STANBRO M., TOELGE K., VERES P.
	Astrophys. J., 826L, 6-6 (2016)
	Fermi GBM observations of LIGO gravitational-wave event GW150914.
o	<[CBG2016] GW150914-GBM> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBH2004]
[CBH2004]	(Cowie+Barger+Hu+, 2004)
Write:	<<[CBH2004] DDD.dddddd+DD.ddddd>>
N:	1604
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Hawaii sample of galaxies in the ACS-GOODS region surrounding the HDFN. The spectra were obtained with either the DEIMOS or LRIS spectrographs on the Keck 10m telescopes.
in source:	NAME GOODS North Field
Ref:	=2004AJ....127.3137C
by	COWIE L.L. , BARGER A.J., HU E.M., CAPAK P., SONGAILA A.
	Astron. J., 127, 3137-3145 (2004)
	A large sample of spectroscopic redshifts in the ACS-GOODS region of the Hubble Deep Field North.
o	Tables 1, 2: <[CBH2004] DDD.dddddd+DD.ddddd> N=1324.
=E=	Catalogue in electronic form as J/AJ/127/3137
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBH2007]
[CBH2007]	(Cyganowski+Brogan+Hunter, 2007)= (SMA)
Write:	<<[CBH2007] SMAN>>
N:	3
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SMA observations of Sh 2-255N.
in source:	SH 2-255 N
Ref:	=2007AJ....134..346C
by	CYGANOWSKI C.J. , BROGAN C.L., HUNTER T.R.
	Astron. J., 134, 346-358 (2007)
	Evidence for a massive protocluster in S255N.
o	Table 3: components SMA1-WW and WW are not in SIMBAD.
o	Table 1: <[CBH2007] SMAN> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBH2010]
[CBH2010]	(Cowie+Barger+Hu, 2010)= (GALEX)
Write:	<<[CBH2010] GALEXHHMM+DDMM>> <<[CBH2010] DDD.dddddd+DD.dddddd>>
N:	438+427
Object:	G (SIMBAD class: Galaxy)
Note:	GALEX grism spectroscopy of nine deep fields.
Ref:	=2010ApJ...711..928C
by	COWIE L.L. , BARGER A.J., HU E.M.
	Astrophys. J., 711, 928-958 (2010)
	Low-redshift Lyα selected galaxies from GALEX spectroscopy: a comparison with both UV-continuum selected galaxies and high-redshift Lyα emitters.
o	Tables 2-16: <[CBH2010] GALEXHHMM+DDMM> N=438. Tables 2-13,15-16: <[CBH2010] DDD.dddddd+DD.dddddd> N=427.
Ref:	=2011ApJ...738..136C
by	COWIE L.L. , BARGER A.J., HU E.M.
	Astrophys. J., 738, 136 (2011)
	Lyα emitting galaxies as early stages in galaxy formation.
o	Table 4, col(1): <[CBH2011] NNN> (Nos 1-100). Tables 1-4: <[CBH2010] DDD.dddddd+DD.dddddd> N=61+32+8+100 added.
=E=	Catalogue in electronic form as <J/ApJ/711/928/>
=E=	Catalogue in electronic form as <J/ApJ/738/136/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBH2011]
[CBH2011]	(Cowie+Barger+Hu, 2011)= ([CBH2011a])
Write:	<<[CBH2011] NNN>>
N:	100
Object:	LAE G (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	Keck II DEIMOS optical spectroscopy of N=100 GALEX grism selected Lymanα emitters. See also [CBH2010].
Ref:	=2011ApJ...738..136C
by	COWIE L.L. , BARGER A.J., HU E.M.
	Astrophys. J., 738, 136 (2011)
	Lyα emitting galaxies as early stages in galaxy formation.
o	Table 4, col(1): <[CBH2011] NNN> (Nos 1-100). Tables 1-4: <[CBH2010] DDD.dddddd+DD.dddddd> N=61+32+8+100 added.
=E=	Catalogue in electronic form as <J/ApJ/738/136/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBH2011a]
[CBH2011a]	(Cowie+Barger+Hu, 2011)
*****	Avoid the usage of [CBH2011a], prefer [CBH2011]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBH2011b]
[CBH2011b]	(Cyganowski+Brogan+Hunter+, 2011)
Write:	<<[CBH2011b] GBB.bb+L.ll MMNN>> <<[CBH2011b] G11.92-0.61 MMN-CN>>
N:	19+3+3+3+1
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	SMA 1.3mm, CARMA 3mm, and ALMA 1.05mm observations of two GLIMPSE Extended Green objects (EGOs).
in source:	EGO G011.92-0.61
in source:	EGO G019.01-0.03
Ref:	=2011ApJ...729..124C
by	CYGANOWSKI C.J. , BROGAN C.L., HUNTER T.R., CHURCHWELL E., ZHANG Q.
	Astrophys. J., 729, 124 (2011)
	Bipolar molecular outflows and hot cores in glimpse extended green objects (EGOs).
o	Table 2: <[CBH2011b] GBB.bb+L.ll MMN> N=4.
Ref:	=2017MNRAS.468.3694C
by	CYGANOWSKI C.J. , BROGAN C.L., HUNTER T.R., SMITH R., KRUIJSSEN J.M.D., BONNELL I.A., ZHANG Q.
	Mon. Not. R. Astron. Soc., 468, 3694-3708 (2017)
	Simultaneous low- and high-mass star formation in a massive protocluster: ALMA observations of G11.92-0.61.
o	Table 2: <[CBH2011b] G11.92-0.61 MMNN> (Nos MM4-MM19) added, <[CBH2011b] G11.92-0.61 MMN-CN> (Nos MM1-C1 to MM1-C3, MM2-C1 to MM2-C3, MM3-C1 to MM3-C3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBH2011c]
[CBH2011c]	(Cyganowski+Brogan+Hunter+, 2011)
Write:	<<[CBH2011c] EGO GLL.ll+B.bb-CMN>> <<[CBH2011c] F GLL.ll+B.bb-CMN>>
N:	12+12
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	EVLA 1.3cm and 3.6cm continuum observations of Extended Green Objects (EGO).
Ref:	=2011ApJ...743...56C
by	CYGANOWSKI C.J. , BROGAN C.L., HUNTER T.R., CHURCHWELL E.
	Astrophys. J., 743, 56 (2011)
	Deep very large array radio continuum surveys of GLIMPSE extended green objects (EGOs).
o	Fig. 1, Table 2: <[CBH2011c] EGO GLL.ll+B.bb-CMN> N=12. Fig. 2, Table 4: <[CBH2011c] F GLL.ll+B.bb-CMN> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBH2015]
[CBH2015]	(Chang+Byun+Hartman, 2015)
Write:	<<[CBH2015] VNNNN>>
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Catalog of N=2306 variable stars in the field of M37. Use of archival MMT transit survey data.
in source:	M 37 = NGC 2099
Ref:	=2015AJ....150...27C
by	CHANG S.-W. , BYUN Y.-I., HARTMAN J.D.
	Astron. J., 150, 27 (2015)
	A new catalog of variable stars in the field of the open cluster M37.
o	Table 1: <[CBH2015] VNNNN> (Nos V1-V2306).
o	Table 1, col(VarID): V1-V1454 are <Cl* NGC 2099 HGH VNNNN> (Nos V1-V1454) in SIMBAD, V1455-V1483 are <Cl* NGC 2099 HGH SNN> (Nos S1-S29) in SIMBAD.
=E=	Catalogue in electronic form as <J/AJ/150/27/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBH2017]
[CBH2017]	(Cowie+Barger+Hsu+, 2017)
Write:	<<[CBH2017] SMM JHHMMSS+DDMMSS>> <<[CBH2017] SMA JHHMMSS+DDMMSS>> <<[CBH2017] SMMHHMMSSDDMMSS>> (not recognised by Simbad, but found in literature) <<[CBH2017] SMAHHMMSSDDMMSS>>
N:	33+186+31
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	JCMT SCUBA-2 850µm and 450µm observations of N=186+31 sources respectively and SMA observations of N=33 sources, in the GOODS-North field. Additional VLA observations at 20cm. See also [CGB2018] for ALMA sources in the GOODS-South field.
in source:	NAME GOODS-N Field
Ref:	=2017ApJ...837..139C
by	COWIE L.L. , BARGER A.J., HSU L.-Y., CHEN C.-C., OWEN F.N., WANG W.-H.
	Astrophys. J., 837, 139-139 (2017)
	A SUbmillimeter PERspective on the GOODS fields (SUPER GOODS). I. An ultradeep SCUBA-2 survey of the GOODS-N.
o	Table 3: <[CBH2017] SMA JHHMMSS+DDMMSS> N=33. Tables 5-6: <[CBH2017] SMM JHHMMSS+DDMMSS> N=186+31.
=E=	Catalogue in electronic form as <J/ApJ/837/139/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBI2003]
[CBI2003]	(Chapman+Balin+Ivison+, 2003)= (SMM)
Write:	<<[CBI2003] SMM JHHMMSS.s+DDMMSS>>
N:	10
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Ref:	=2003Natur.422..695C
by	CHAPMAN S.C. , BLAIN A.W., IVISON R.J., SMAIL I.R.
	Nature, 422, 695-698 (2003)
	A median redshift of 2.4 for galaxies bright at submillimetre wavelengths.
o	Table 1: <[CBI2003] SMM JHHMMSS.s+DDMMSS> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBI2009]
[CBI2009]	(Chapman+Blain+Ibata +, 2009)
Write:	<<[CBI2009] SCBX-NNNN>> <<[CBI2009] z1.99 Cluster>>
N:	2+1
Object:	G + CLuster of G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=2 UV-selected galaxies around z=2 and N=1 high-z cluster of submillimeter galaxies in the GOODS-N field.
in source:	NAME GOODS North Field
Ref:	=2009ApJ...691..560C
by	CHAPMAN S.C. , BLAIN A., IBATA R., IVISON R.J., SMAIL I., MORRISON G.
	Astrophys. J., 691, 560-568 (2009)
	Do submillimeter galaxies really trace the most massive dark-matter halos? Discovery of a high-z cluster in a highly active phase of evolution.
o	Table 1: <[CBI2009] SCBX-NNNN> (Nos 6106, 6946). Text: <[CBI2009] z1.99 cluster> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBI89]
[CBI89]	(Cristiani+Barbieri+Iovino+, 1989) (Not yet in Simbad)
Write:	<<[CBI89] {Q\|S\|H}HHMM+DDMMA>> <<[CBI89] HHMM+DDMMA>>
N:	80+14+5+123
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Sample of QSOs.: First letter in the format is Q (QSO), S (seyfert) or H (HII). Other objects have a format not beginning by a letter.
Ref:	=1989A&AS...77..161C
by	CRISTIANI S. , BARBIERI C., IOVINO A., LA FRANCA F., NOTA A.
	Astron. Astrophys., Suppl. Ser., 77, 161-207 (1989)
	Quasars in the field of SA 94. III. A colour survey.
o	Table II: <[CBI89] AHHMM+DDMMA> N=80+14+5. Table III: <[CBI89] HHMM+DDMMA> N=123.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBJ2002]
[CBJ2002]	(Cambresy+Beichman+Jarrett+, 2002)= (CBJC)
Write:	<<[CBJ2002] Na>>
N:	9
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	Discovery of stellar clusters toward the North America Nebula.
Ref:	=2002AJ....123.2559C
by	CAMBRESY L. , BEICHMAN C.A., JARRETT T.H., CUTRI R.M.
	Astron. J., 123, 2559-2573 (2002)
	Extinction with 2MASS: star counts and reddening toward the North America and Pelican nebulae.
o	Table 1, Fig.11: <[CBJ2002] Na> (Nos 1-2, 3a-3b, 4-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBJ2012]
[CBJ2012]	(Casewell+Baker+Jameson+, 2012)
Write:	<<[CBJ2012] blNNNNN-NNNNN>>
N:	44
Object:	Poss. Low-mass * (SIMBAD class: Low-Mass*_Candidate = Low-mass Star Candidate)
Note:	UKIRT WFCAM NIR observations of N=44 candidate low-mass stellar and substellar members of the young open cluster Cl Blanco 1. Use of previous CFHT CFH12k observations by Morux et al. (2007A&A...471..499M, see [MBS2007b]).
in source:	Cl Blanco 1
Ref:	=2012MNRAS.425.3112C
by	CASEWELL S.L. , BAKER D.E.A., JAMESON R.F., HODGKIN S.T., DOBBIE P.D., MORAUX E.
	Mon. Not. R. Astron. Soc., 425, 3112-3118 (2012)
	A photometric and astrometric investigation of the brown dwarfs in blanco 1.
o	Table 1: <[CBJ2012] blNNNNN-NNNNN> N=44.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBJ2019]
[CBJ2019]	(Chen+Boettcher+Johnson+, 2019)
Write:	<<[CBJ2019] JHHMMSS.ss+DDMMSS.ss>>
N:	14
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Archival HST WFPC2 and VLT MUSE observations of N=14 galaxies in the field of PKS 1127-145.
Ref:	=2019ApJ...878L..33C
by	CHEN H.-W. , BOETTCHER E., JOHNSON S.D., ZAHEDY F.S., RUDIE G.C., COOKSEY K.L., RAUCH M., MULCHAEY J.S.
	Astrophys. J., 878L, 33-33 (2019)
	A giant intragroup nebula hosting a damped Lyαabsorber at z = 0.313.
o	Figs 1+3, Table 1: <[CBJ2019] JHHMMSS.ss+DDMMSS.ss> N=14.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBJ88]
[CBJ88]	(Cohen+Baart+Jonas, 1988)
Write:	<<[CBJ88] HHMMSS.s+DDMMSS>>
N:	17
Object:	OH Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	N=17 new OH masers associated with 17 IRAS sources.
Ref:	=1988MNRAS.231..205C
by	COHEN R.J. , BAART E.E., JONAS J.L.
	Mon. Not. R. Astron. Soc., 231, 205-227 (1988)
	OH masers associated with IRAS far-infrared sources.
o	(Erratum) + erratum vol. 240, 255
o	Table 1: <[CBJ88] HHMMSS.s+DDMMSS> N=17.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CBJC
CBJC	(Cambresy+Beichman+Jarrett+Cutri)
*****	Avoid the usage of CBJC, prefer [CBJ2002]
Origin	of the Acronym: L (2003A&A...397..177B)
Details on Acronym: [CBK2001]
[CBK2001]	(Collinge+Brandt+Kaspi+, 2001)
Write:	<<[CBK2001] JHHMMSS.ss+DDMMSS.s>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	HETGS Chandra observations of NGC 4051. Discovery of two weak off-nuclear sources coincident with the galactic disk of NGC 4051.
Ref:	=2001ApJ...557....2C
by	COLLINGE M.J. , BRANDT W.N., KASPI S., CRENSHAW D.M., ELVIS M., KRAEMER S.B., REYNOLDS C.S., SAMBRUNA R.M., WILLS B.J.
	Astrophys. J., 557, 2-17 (2001)
	High-resolution X-ray and ultraviolet spectroscopy of the complex intrinsic absorption in NGC 4051 with Chandra and the Hubble space telescope.
o	Text: <[CBK2001] JHHMMSS.ss+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBK2002]
[CBK2002]	(Cowie+Barger+Kneib, 2002)
Write:	<<[CBK2002] CN>> <<[CBK2002] NN>>
N:	5+15
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	850microm. maps of the lensing clusters, ACO 370, ACO 851, ACO 2390. Table 2: (Nos C0-C4): cluster submillimeter sources. Table 3: (Nos 0-14): background submillimeter sources.
in source:	ACO 370
in source:	ACO 851 = ClG 0939+4713
in source:	ACO 2390
Ref:	=2002AJ....123.2197C
by	COWIE L.L. , BARGER A.J., KNEIB J.-P.
	Astron. J., 123, 2197-2205 (2002)
	Faint submillimeter counts from deep 850 micron observations of the lensing clusters A370, A851, and A2390.
o	Table 2: <[CBK2002] CN> (Nos C0-C4). Table 3: <[CBK2002] NN> (Nos 0-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBK2007]
[CBK2007]	(Chien+Barnes+Kewley+, 2007)= ([CBK2007a])
Write:	<<[CBK2007] SNNa>>
N:	10+3
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	Keck I LRIS spectroscopy of NGC 4676.
in source:	NGC 4676 = Mice
Ref:	=2007ApJ...660L.105C
by	CHIEN L.-H. , BARNES J.E., KEWLEY L.J., CHAMBERS K.C.
	Astrophys. J., 660L, 105-108 (2007)
	Multiobject spectroscopy of young star clusters in NGC 4676.
o	Table 1: <[CBK2007] SNNa> (Nos S1-S10, S4a, S9a-S9b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBK2007a]
[CBK2007a]	(Chien+Barnes+Kewley+, 2007)
*****	Avoid the usage of [CBK2007a], prefer [CBK2007]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBK2007b]
[CBK2007b]	(Currie+Balog+Kenyon+, 2007)
Write:	<<[CBK2007b] DD.dddd+DD.dddd>>
N:	31265
Object:	* in stellar cluster (SIMBAD class: Star)
Note:	Spitzer IRAC and 1.8m Perkins telescope at Lowell Observatory NIR observations of the double cluster h and chi Persi. Use of archival 2MASS data. See also [CKR2007], [CKB2008].
in source:	NAME h Per = NGC 869
in source:	NAME khi Per = NGC 884
Ref:	=2007ApJ...659..599C
by	CURRIE T. , BALOG Z., KENYON S.J., RIEKE G., PRATO L., YOUNG E.T., MUZEROLLE J., CLEMENS D.P., BUIE M., SARCIA D., GRABU A., TOLLESTRUP E.V., TAYLOR B., DUNHAM E., MACE G.
	Astrophys. J., 659, 599-615 (2007)
	Spitzer IRAC and JHK_{s} observations of h and χ Persei: constraints on protoplanetary disk and massive cluster evolution at ~10^{7} years.
o	Table 2: <[CBK2007b] DD.dddd+DD.dddd> N=31265
=E=	Catalogue in electronic form as J/ApJ/659/599
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBK2016]
[CBK2016]	(Coude+Bastien+Kirk+, 2016)
Write:	<<[CBK2016] CNN>>
N:	33
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	JCMT SCUBA-2 450µm and 850µm observations of N=33 smm sources in Ori A molecular cloud.
in source:	NAME Ori A
Ref:	=2016MNRAS.457.2139C
by	COUDE S. , BASTIEN P., KIRK H., JOHNSTONE D., DRABEK-MAUNDER E., GRAVES S., HATCHELL J., CHAPIN E.L., GIBB A.G., MATTHEWS B., (The JCMT Gould Belt Survey Team)
	Mon. Not. R. Astron. Soc., 457, 2139-2150 (2016)
	The JCMT Gould Belt Survey: the effect of molecular contamination in SCUBA-2 observations of Orion A.
o	Table 1: <[CBK2016] CNN> (Nos C01-C33).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBL2018]
[CBL2018]	(Chen+Brandt+Luo+, 2024) (Not yet in Simbad)
Write:	<<[CBL2018] XMMNNNNN>>
N:	5242
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton observations of N=5242 X-ray sources in the XMM-Large Scale Structure (XMM-LSS) field, as part of the XMM-Spitzer Extragalactic Representative Volume Survey (XMM-SERVS) survey. For more information, visit: https://personal.science.psu.edu/wnb3/xmmservs/xmmservs.html See also [NBC2021] for sources in the W-CDF-S and ELAIS-S1 fields.
in source:	NAME XMM-LSS Field
Ref:	=2018MNRAS.478.2132C
by	CHEN C.-T.J. , BRANDT W.N., LUO B., RANALLI P., YANG G., ALEXANDER D.M., BAUER F.E., KELSON D.D., LACY M., NYLAND K., TOZZI P., VITO F., CIRASUOLO M., GILLI R., JARVIS M.J., LEHMER B.D., PAOLILLO M., SCHNEIDER D.P., SHEMMER O., SMAIL I., SUN M., TANAKA M., VACCARI M., VIGNALI C., XUE Y.Q., BANERJI M., CHOW K.E., HAUSSLER B., NORRIS R.P., SILVERMAN J.D., TRUMP J.R.
	Mon. Not. R. Astron. Soc., 478, 2132-2163 (2018)
	The XMM-SERVS survey: new XMM-Newton point-source catalogue for the XMM-LSS field.
o	Table A: <[CBL2018] XMMNNNNN> (Nos XMM00000-XMM05241).
=E=	Catalogue in electronic form as <J/MNRAS/478/2132/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [CBM2000]
[CBM2000]	(Centurion+Bonifacio+Molaro+, 2000)
Write:	<<[CBM2000] QSO JHHMM+DDMM abs N.NNN>> <<[CBM2000] QSO JHHMM+DDMM abs N.NNNN>>
N:	7
Object:	Absorber
Note:	ESO 3.6m telescope and WHT observations. N=7 absorption systems in the line of sight of 6 QSOs.
Ref:	=2000ApJ...536..540C
by	CENTURION M. , BONIFACIO P., MOLARO P., VLADILO G.
	Astrophys. J., 536, 540-549 (2000)
	Chemical evolution of damped Lyα galaxies: the [S/Zn] abundance ratio at redshift ≥2.
o	Table 1: <[CBM2000] QSO JHHMM+DDMM abs N.NNN> N=1, <[CBM2000] QSO JHHMM+DDMM abs N.NNNN> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBM2013]
[CBM2013]	(Carraro+Beletsky+Marconi, 2013)
Write:	<<[CBM2013] Berkeley 76 NNNN>> <<[CBM2013] Haffner NN NNNN>> <<[CBM2013] Ruprecht 10 NNNN>>
N:	3433+8118+3330+6078+8319+7342+5396
Object:	* (SIMBAD class: Star)
Note:	CTIO 1.0m telescope observations of open clusters in the outer Galactic disc.
in source:	Cl Berkeley 76
in source:	Cl Haffner 4
in source:	Cl Haffner 7
in source:	Cl Haffner 11
in source:	Cl Haffner 15
in source:	Cl Ruprecht 10
Ref:	=2013MNRAS.428..502C
by	CARRARO G. , BELETSKY Y., MARCONI G.
	Mon. Not. R. Astron. Soc., 428, 502-517 (2013)
	Five old open clusters more in the outer Galactic disc.
o	<[CBM2013] Berkeley 76 NNNN> (Nos 1-3433), <[CBM2013] Haffner NN NNNN> N=6078+8319+7342+8118+3330, <[CBM2013] Ruprecht 10 NNNN> (Nos 1-5396).
o	In references, Carraro et al. 2008, MNRAS, 383, 1597 is a misprint for Carraro et al. 2008, MNRAS, 385, 1597 (2008MNRAS.385.1597C).
=E=	Catalogue in electronic form as <J/MNRAS/428/502/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBM2016]
[CBM2016]	(Chan+Beifiori+Mendel+, 2016)
Write:	<<[CBM2016] NNN>>
N:	36
Object:	G (SIMBAD class: Galaxy)
Note:	N=36 passive galaxies in the XMMUJ2235-2557 cluster at z∼1.39. Use of archival HST ACS/WFC3 images. See also [SGC2017].
in source:	ClG J2235-2557
Ref:	=2016MNRAS.458.3181C
by	CHAN J.C.C. , BEIFIORI A., MENDEL J.T., SAGLIA R.P., BENDER R., FOSSATI M., GALAMETZ A., WEGNER M., WILMAN D.J., CAPPELLARI M., DAVIES R.L., HOUGHTON R.C.W., PRICHARD L.J., LEWIS I.J., SHARPLES R., STOTT J.P.
	Mon. Not. R. Astron. Soc., 458, 3181-3209 (2016)
	Sizes, colour gradients and resolved stellar mass distributions for the massive cluster galaxies in XMMUJ2235-2557 at z = 1.39.
o	Table F1: <[CBM2016] NNN> N=36 among (Nos 36-642).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBM2023]
[CBM2023]	(Carnall+Begley+McLeod+, 2023)
Write:	<<[CBM2023] NNNNN>> <<[CBM2023] sNNNNN>> (not recognised by Simbad, but found in literature)
N:	10
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	JWST NIRSpec MSA observations of N=10 galaxies in the SMACS J0723.3-7327 cluster field. The object ID numbers come from the input source catalog used for the JWST NIRSpec micro-shutter-array (MSA) configuration planning. Only the first reference citing these numbers is listed here.
in source:	SMACS J0723.3-7327
Ref:	=2023MNRAS.518L..45C
by	CARNALL A.C. , BEGLEY R., McLEOD D.J., HAMADOUCHE M.L., DONNAN C.T., McLURE R.J., DUNLOP J.S., MILVANG-JENSEN B., BONDESTAM C.L., CULLEN F., JEWELL S.M., POLLOCK C.L.
	Mon. Not. R. Astron. Soc., 518L, 45-50 (2023)
	A first look at the SMACS0723 JWST ERO: spectroscopic redshifts, stellar masses, and star-formation histories.
o	Tables 1-2: <[CBM2023] NNNNN> N=10 among (Nos 1917-10612).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: CBN
CBN	(Corti+Bosch+Niemela)
*****	Avoid the usage of CBN, prefer [CBN2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CBN2001]
[CBN2001]	(Codella+Bachiller+Nisini+, 2001)
Write:	<<[CBN2001] A>> <<[CBN2001] W Outflow>>
N:	3+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Fig.1: N=3 continuum sources (Nos A-C). Table 3: N=2 outflows, Northern and Central. See also [NMV2001].
in source:	IC 1396N
Ref:	=2001A&A...376..271C
by	CODELLA C. , BACHILLER R., NISINI B., SARACENO P., TESTI L.
	Astron. Astrophys., 376, 271-287 (2001)
	Star formation in the bright rimmed globule IC 1396N.
o	Fig.1: <[CBN2001] A> (Nos A-C). Table 3: <[CBN2001] W Outflow> (Nos N, C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBN2007]
[CBN2007]	(Corti+Bosch+Niemela, 2007)
Write:	<<[CBN2007] JHHMMSS.s+DDMMSS>>
N:	64+10
Object:	* In Assoc (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	CTIO 1-m Curtis Schmidt telescope observations of Bochum 7.
in source:	Cl Bochum 7
Ref:	=2007A&A...467..137C
by	CORTI M. , BOSCH G., NIEMELA V.
	Astron. Astrophys., 467, 137-143 (2007)
	A search for OB stars in the field of the galactic OB association Bochum 7. I. UBV-IR photometry and optical spectroscopy.
o	[CBN2007] J084437.8-455257 is 2MASS J08443780-4552564
o	Table 1: <[CBN2007] JHHMMSS.s+DDMMSS> N=64.
Ref:	=2018A&A...616A..40C
by	CORTI M.A. , ORELLANA R.B., BOSCH G.L.
	Astron. Astrophys., 616A, 40-40 (2018)
	A search for OB stars in the field of the galactic OB association Bochum 7. II. Proper motion and IR photometry.
o	Tables 1-3: <[COB2018] NNNN> N=248 among (Nos 7-4903). Table 2: <[CBN2007] JHHMMSS.s+DDMMSS> N=10 added.
=E=	Catalogue in electronic form as <J/A+A/616/A40/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBO2001]
[CBO2001]	(Carilli+Bertoldi+Omont+, 2001)
Write:	<<[CBO2001] JHHMMSS.ss+DDMMSS.s>> <<[CBO2001] JHHMMSS.s+DDMMSS.ss>>
N:	6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA observations of radio-sources near QSOs.
Ref:	=2001AJ....122.1679C
by	CARILLI C.L. , BERTOLDI F., OMONT A., COX P., McMAHON R.G., ISAAK K.G.
	Astron. J., 122, 1679-1687 (2001)
	Radio observations of infrared-luminous high-redshift quasi-stellar objects.
o	Text, 3.1: <[CBO2001] JHHMMSS.ss+DDMMSS.s>, <[CBO2001] JHHMMSS.ss+DDMMSS.s>, N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBP2011]
[CBP2011]	(Clements+Bendo+Pearson+, 2011)
Write:	<<[CBP2011] SST24 NNNNN>> <<[CBP2011] SST70 NNNN>>
N:	41503+1203
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Spitzer (SST) 24 and 70µm observations of the Akari Deep Field-South (ADF-S).
Ref:	=2011MNRAS.411..373C
by	CLEMENTS D.L. , BENDO G., PEARSON C., KHAN S.A., MATSUURA S., SHIRAHATA M.
	Mon. Not. R. Astron. Soc., 411, 373-384 (2011)
	The AKARI Deep Field-South: Spitzer 24- and 70-µm observations, catalogues and counts.
o	Table 3: <[CBP2011] SST24 NNNNN> (Nos 0-41502). Table 4: <[CBP2011] SST70 NNNN> (Nos 0-1202).
o	DC 0428-43 is a probable misprint for DC 0428-53
=E=	Catalogue in electronic form as J/MNRAS/411/373
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBP2015]
[CBP2015]	(Cappellaro+Botticella+Pignata+, 2015)
Write:	<<[CBP2015] {cdfs}{1\|2} {r} YYYYMMDD NNNA>> <<[CBP2015] cosmos r YYYYMMDD NNNA>>
N:	117
Object:	SN (SIMBAD class: Supernova = SuperNova)
Note:	VST-OmegaCAM observations of N=117 supernovae in the CDFS and COSMOS fields. Use of images from the SUpernova Diversity And Rate Evolution (SUDARE) survey.
in source:	NAME COSMOS Field
in source:	NAME Chandra Deep Field-South
Ref:	=2015A&A...584A..62C
by	CAPPELLARO E. , BOTTICELLA M.T., PIGNATA G., GRADO A., GREGGIO L., LIMATOLA L., VACCARI M., BARUFFOLO A., BENETTI S., BUFANO F., CAPACCIOLI M., CASCONE E., COVONE G., DE CICCO D., FALOCCO S., DELLA VALLE M., JARVIS M., MARCHETTI L., NAPOLITANO N.R., PAOLILLO M., PASTORELLO A., RADOVICH M., SCHIPANI P., SPIRO S., TOMASELLA L., TURATTO M.
	Astron. Astrophys., 584A, 62-62 (2015)
	Supernova rates from the SUDARE VST-OmegaCAM search. I. Rates per unit volume.
o	Table A.2: <[CBP2015] cdfs1 r YYYYMMDD NNNA> N=39, <[CBP2015] cdfs2 r YYYYMMDD NNNA> N=41, <[CBP2015] cosmos r YYYYMMDD NNNA> N=37.
=E=	Catalogue in electronic form as J/A+A/584/A62
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBP2016]
[CBP2016]	(Clements+Braglia+Petitpas+, 2016)
Write:	<<[CBP2016] LABOCA N>> <<[CBP2016] SCUBA2 NN>>
N:	7+14
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	APEX LABOCA 870µm and JCMT SCUBA-2 850µm observations of N=7+14 submillimetre sources in the field of [BPA2013] H-ATLAS J114637.9-001132 lens.
Ref:	=2016MNRAS.461.1719C
by	CLEMENTS D.L. , BRAGLIA F., PETITPAS G., GREENSLADE J., COORAY A., VALIANTE E., DE ZOTTI G., O'HALLORAN B., HOLDSHIP J., MORRIS B., PEREZ-FOURNON I., HERRANZ D., RIECHERS D., BAES M., BREMER M., BOURNE N., DANNERBAUER H., DARIUSH A., DUNNE L., EALES S., FRITZ J., GONZALEZ-NUEVO J., HOPWOOD R., IBAR E., IVISON R.J., LEEUW L.L., MADDOX S., MICHALOWSKI M.J., NEGRELLO M., OMONT A., OTEO I., SERJEANT S., VALTCHANOV I., VIEIRA J.D., WARDLOW J., VAN DER WERF P.
	Mon. Not. R. Astron. Soc., 461, 1719-1733 (2016)
	H-ATLAS: a candidate high redshift cluster/protocluster of star-forming galaxies.
o	Fig. 1, Table 1: <[CBP2016] LABOCA N> (Nos 1-7). Fig. 1, Table 2: <[CBP2016] SCUBA2 NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBR2002]
[CBR2002]	(Cotter+Buttery+Rawlings+, 2002)
Write:	<<[CBR2002] JHHMMSS.ss+DDMMSS.ss>> <<[CBR2002] A>>
N:	8
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=8 radio-sources toward the TOC cluster ClG J0233+3021. Among these radio-sources, 5 are NVSS sources, and are radio galaxies.
in source:	ClG J0233+3021
Ref:	=2002MNRAS.331....1C
by	COTTER G. , BUTTERY H.J., RAWLINGS S., CROFT S., HILL G.J., GAY P., DAS R., DRORY N., GRAINGE K., GRAINGER W.F., JONES M.E., POOLEY G.G., SAUNDERS R.
	Mon. Not. R. Astron. Soc., 331, 1-6 (2002)
	Detection of a cosmic microwave background decrement towards a cluster of mJy radio sources.
o	TOC J0233.3+3021 = ClG J0233+3021
o	Fig.2: <[CBR2002] A> (Nos A-E). <[CBR2002] JHHMMSS.ss+DDMMSS.ss> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBR2007]
[CBR2007]	(Cantiello+Blakeslee+Raimondo+, 2007)
Write:	<<[CBR2007] JHHMMSS.ss+DDMMSS.ss>>
N:	109
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Note:	HST ACS survey of NGC 5866. Search for globular clusters.
in source:	NGC 5866
Ref:	=2007ApJ...668..209C
by	CANTIELLO M. , BLAKESLEE J.P., RAIMONDO G.
	Astrophys. J., 668, 209-220 (2007)
	The globular cluster system in NGC 5866: optical observations from Hubble Space Telescope Advanced Camera for Surveys.
o	Table 1: <[CBR2007] JHHMMSS.ss+DDMMSS.ss> N=109.
=E=	Catalogue in electronic form as J/ApJ/668/209
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBR2013]
[CBR2013]	(Caso+Bassino+Richtler+, 2013)= (ACO)
Write:	<<[CBR2013] ACO NN>>
N:	35
Object:	G (SIMBAD class: Galaxy)
Note:	VLT FORS1, CTIO MOSAIC and Gemini GMOS observations of N=35 compact objects in the Antlia galaxy cluster. Use of HST ACS archival data.
in source:	NAME Antlia Cluster
Ref:	=2013MNRAS.430.1088C
by	CASO J.P. , BASSINO L.P., RICHTLER T., SMITH CASTELLI A.V., FAIFER F.R.
	Mon. Not. R. Astron. Soc., 430, 1088-1101 (2013)
	Ultracompact dwarfs around NGC3258 in the Antlia cluster.
o	W3 in NGC 7252 = [WSL93] 3 ; UCD 3 = [DJG2000] UCO 3 ; VUCD 7 = [JDJ2006] 7 ; FS90-NNN = [FS90] Antlia NNN.
o	Table 1: <[CBR2013] ACO NN> (Nos 1-11).
Ref:	=2014MNRAS.442..891C
by	CASO J.P. , BASSINO L.P., RICHTLER T., CALDERON J.P., SMITH CASTELLI A.V.
	Mon. Not. R. Astron. Soc., 442, 891-899 (2014)
	Ultracompact dwarfs around NGC 3268.
o	Table 1: <[CBR2013] ACO NN> (Nos 12-35) added. Table 2: <[CBR2014] JHHMMSS.ss+DDMMSS.ss> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBR2014]
[CBR2014]	(Caso+Bassino+Richtler+, 2014)
Write:	<<[CBR2014] JHHMMSS.ss+DDMMSS.ss>>
N:	9
Object:	Extended cluster (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS1 and CTIO 4m telescope MOSAIC photometry and Gemini GMOS spectroscopy of N=2+7 extended clusters (EC) around NGC 3268 and near NGC 3258.
in source:	NGC 3268
in source:	NGC 3258
Ref:	=2014MNRAS.442..891C
by	CASO J.P. , BASSINO L.P., RICHTLER T., CALDERON J.P., SMITH CASTELLI A.V.
	Mon. Not. R. Astron. Soc., 442, 891-899 (2014)
	Ultracompact dwarfs around NGC 3268.
o	Table 1: <[CBR2013] ACO NN> (Nos 12-35) added. Table 2: <[CBR2014] JHHMMSS.ss+DDMMSS.ss> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CBS
CBS	(Case univ., Blue *)
Write:	<<CBS NNN>>
N:	465
Object:	Blue * (SIMBAD class: Star)
Note:	Identif. charts.
Ref:	=1983ApJS...51..171P
by	PESCH P. , SANDULEAK N.
	Astrophys. J., Suppl. Ser., 51, 171-182 (1983)
	The Case low-dispersion northern sky survey. I.
o	Table 1: <CasG NN> (Nos 1-71), Table 1A: <CasHII Z FFF-NNN a> N=4, Table 2: <CSO NN> (Nos 1-59), Table 3: <CBS NN> (Nos 1-28)
Ref:	=1984ApJS...55..517S
by	SANDULEAK N. , PESCH P.
	Astrophys. J., Suppl. Ser., 55, 517-532 (1984)
	The Case low-dispersion northern sky survey. II.
o	(Erratum) Erratum 1996 ApJS 103, p. 513
o	Table 1: <CasG NNN> (Nos 72-196), Table 1A: <CasHII Z FFF-NNN a> N=40, Table 2: <CSO NNN> (Nos 60-179), Table 3: <CBS NN> (Nos 29-66)
Ref:	=1986ApJS...60..543P
by	PESCH P. , SANDULEAK N.
	Astrophys. J., Suppl. Ser., 60, 543-549 (1986)
	The Case low-dispersion northern sky survey. III.
o	Table 1: <CasG NNN> (Nos 197-326), Table 1A: <CasHII Z FFF-NNN a> N=6, <CasHII HHMMSS.s+DDMM.m a> N=1, Table 2: <CSO NNN> (Nos 180-252), Table 3: <CBS NNN> (Nos 67-124)
Ref:	=1988ApJS...66..297P
by	PESCH P. , SANDULEAK N.
	Astrophys. J., Suppl. Ser., 66, 297-307 (1988)
	The Case low-dispersion northern sky survey. V.
o	Table 1: <CasG NNN> (Nos 753-895), Table 1A: <CasHII Z FFF-NNN a> N=20, <CasHII HHMMSS.s+DDMM.m a> N=3, Table 2: <CSO NNN> (Nos 253-401), Table 3: <CBS NNN> (Nos 125-160)
Ref:	=1989ApJS...70..163P
by	PESCH P. , SANDULEAK N.
	Astrophys. J., Suppl. Ser., 70, 163-171 (1989)
	The Case low-dispersion northern sky survey. VIII. A region centered in southern Bootes.
o	Table 1: <CasG NNN> (Nos 896-907), Table 2: <CSO NNN> (Nos 402-602), Table 3: <CBS NNN> (Nos 161-252)
Ref:	=1989ApJS...70..173S
by	SANDULEAK N. , PESCH P.
	Astrophys. J., Suppl. Ser., 70, 173-179 (1989)
	The Case low-dispersion northern sky survey. IX. A region centered in northern Bootes.
o	Table 1: <CasG NNN> (Nos 908-925), Table 2: <CSO NNN> (Nos 603-765), Table 3: <CBS NNN> (Nos 253-324)
Ref:	=1990ApJS...72..291S
by	SANDULEAK N. , PESH P.
	Astrophys. J., Suppl. Ser., 72, 291-301 (1990)
	The Case low-dispersion northern sky survey. XI. A region near the North Galactic Pole including SA 57.
o	Table 1: <CasG NNNN> (Nos 926-1019), Table 2: <CSO NNN> (Nos 766-881), Table 3: <CBS NNN> (Nos 325-350)
Ref:	=1991ApJS...76.1043P
by	PESCH P. , SANDULEAK N., STEPHENSON C.B.
	Astrophys. J., Suppl. Ser., 76, 1043-1053 (1991)
	The Case low-dispersion northern sky survey. XII. A region in southern Canes Venatici.
o	(Erratum) Erratum 1996 ApJS 102, p. 435, and 1996 ApJS 103, p. 513
o	Table 2: <CasG NNNN> (Nos 1020-1213), Table 3: <CasHII PGC NNNNN>, <CasHII PGC NNNNN a> N=3+12, Table 4: <CSO NNNN> (Nos 882-1038), Table 5: <CBS NNN> (Nos 351-382)
Ref:	=1992ApJS...82..471S
by	STEPHENSON C.B. , PESCH P., MacCONNELL D.J.
	Astrophys. J., Suppl. Ser., 82, 471-487 (1992)
	The case Low-Dispersion Northern Sky Survey. XIII. A region in central Bootes and Corona Borealis.
o	Table 1: <CasG NNNN> (Nos 1214-1351), Table 2:<CasHII PGC NNNNN a> N=4, Table 3: <CSO NNNN> (Nos 1039-1121), Table 4: <CBS NNN> (Nos 383-418)
Ref:	=1995ApJS...98...41P
by	PESCH P. , STEPHENSON C.B., MacCONNELL D.J.
	Astrophys. J., Suppl. Ser., 98, 41-67 (1995)
	The Case low-dispersion northern sky survey. XV. A region in Ursa Major and Canes Venatici.
o	(Erratum) Erratum 1996 ApJS 102, p. 435, and 1996 ApJS 103, p. 513
o	Table 1: <CasG NNNN> (Nos 1352-1579), Table 2: <CasHII PGC NNNNN> <CasHII PGC NNNNN a> <CasHII Anon a> N=7+34+2, Table 4: <CSO NNNN> (Nos 1122-1336), Table 5: <CBS NNN> (Nos 419-465)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CBS2002]
[CBS2002]	(Cohen+Briley+Stetson, 2002)
Write:	<<[CBS2002] CMMSSs+MMSS>>
N:	64
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Keck observations of M 5. Format derived from 2000 coordinates, with RA 15h and Dec +2deg. In 2004AJ....127.1579B, two stars that are misidentified are corrected. See also [BCS2004].
in source:	M 5 = NGC 5904
Ref:	=2002AJ....123.2525C
by	COHEN J.G. , BRILEY M.M., STETSON P.B.
	Astron. J., 123, 2525-2540 (2002)
	Carbon and nitrogen abundances in stars at the base of the red giant branch in M5.
o	Tables 1, 2: Format derived from 2000 coordinates, with RA 15h and Dec +2°. Two stars are misidentified and corrected in 2004AJ....127.1579B
o	Tables 1, 2: <[CBS2002] CMMSSs+MMSS> N=64.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBS2003]
[CBS2003]	(Catanzaro+Bianchi+Scuderi+, 2003)
Write:	<<[CBS2003] M 33 NNN-NN>> <<[CBS2003] NGC 6822 NNN-NN>>
N:	7+3
Object:	* (SIMBAD class: Star)
Note:	New spectroscopy from WHT for a sample of stars in OB associations of two galaxies M 33 and NGC 6822. The authors used a different format for other stars in Paper I: [BCS2001].
in source:	M 33 = NGC 598
in source:	NGC 6822
Ref:	=2003A&A...403..111C
by	CATANZARO G. , BIANCHI L., SCUDERI S., MANCHADO A.
	Astron. Astrophys., 403, 111-117 (2003)
	Spectroscopy of early-type star candidates in M 33 and NGC 6822. II.
o	Table 1: ID LB-f2-977 and LB-f2-999 not corresponding to [BSM2001] LB-f2-NNN where the numbering NNN is from 1 to 260. Could be [BSM2001] LB-f2-215 and [BSM2001] LB-f2-226?
o	Table 1: <[CBS2003] M 33 NNN-NN> N=7, <[CBS2003] NGC 6822 NNN-NN> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBS2005]
[CBS2005]	(Chapman+Blain+Smail+, 2005)= ([CBS2005a]) = (SMM)
Write:	<<[CBS2005] SMM JHHMMSS.ss+DDMMSS.s>>
N:	76+12
Object:	Submm G (SIMBAD class: Galaxy)
Note:	Keck telescope observations of submillimeter galaxies.
Ref:	=2005ApJ...622..772C
by	CHAPMAN S.C. , BLAIN A.W., SMAIL I., IVISON R.J.
	Astrophys. J., 622, 772-796 (2005)
	A redshift survey of the submillimeter galaxy population.
o	In table 2, SMM J141800.40+512820.3 is a misprint for SMM J141800.40+522820.3.
o	Table 2, text: <[CBS2005] SMM JHHMMSS.ss+DDMMSS.s> N=76+12.
=E=	Catalogue in electronic form as J/ApJ/622/772
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBS2005a]
[CBS2005a]	(Chapman+Blain+Smail+, 2005)
*****	Avoid the usage of [CBS2005a], prefer [CBS2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBS2005b]
[CBS2005b]	(Caretti+Bernardi+Sault+, 2005)
Write:	<<[CBS2005b] N>>
N:	9
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA 1.4GHz observations centered on RA 5h, Dec -49deg. N=9 point sources are found.
Ref:	=2005MNRAS.358....1C
by	CARRETTI E. , BERNARDI G., SAULT R.J., CORTIGLIONI S., POPPI S.
	Mon. Not. R. Astron. Soc., 358, 1-12 (2005)
	High Galactic latitude polarized emission at 1.4 GHz and implications for cosmic microwave background observations.
o	Table 2: <[CBS2005b] N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBS2005c]
[CBS2005c]	(Cohen+Briley+Stetson+, 2005)
Write:	<<[CBS2005c] CMMSSs-MMSS>>
N:	73
Object:	* in Cl* (SIMBAD class: Star)
Note:	Keck LRIS observations of stars in M 15 cluster. format: position relative to RA=21h, Dec=+12deg.
in source:	M 15 = NGC 7078
Ref:	=2005AJ....130.1177C
by	COHEN J.G. , BRILEY M.M., STETSON P.B.
	Astron. J., 130, 1177-1193 (2005)
	C and N abundances in stars at the base of the red giant branch in M15.
o	Table 1: <[CBS2005c] CMMSSs-MMSS> N=73.
=E=	Catalogue in electronic form as J/AJ/130/1177
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBS2006]
[CBS2006]	(Coe+Benitez+Sanchez+, 2006)
Write:	<<[CBS2006] NNNNN>>
N:	18700
Object:	G (SIMBAD class: Galaxy)
Note:	Photometry of galaxies in the HUDF.
in source:	NAME HUDF
Ref:	=2006AJ....132..926C
by	COE D. , BENITEZ N., SANCHEZ S.F., JEE M., BOUWENS R., FORD H.
	Astron. J., 132, 926-959 (2006)
	Galaxies in the Hubble Ultra Deep Field. I. Detection, multiband photometry, photometric redshifts, and morphology.
o	Tables 3, 4: <[CBS2006] NNNNN> N=18700 among (Nos 1-60319).
=E=	Catalogue in electronic form as J/AJ/132/926
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBS2007]
[CBS2007]	(Cenarro+Beasley+Strader+, 2007)
Write:	<<[CBS2007] NN>>
N:	21 among 33
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	HST ACS observations of NGC 1407. Search for globular cluster candidates.
in source:	NGC 1407
Ref:	=2007AJ....134..391C
by	CENARRO A.J. , BEASLEY M.A., STRADER J., BRODIE J.P., FORBES D.A.
	Astron. J., 134, 391-410 (2007)
	Stellar populations of globular clusters in the elliptical galaxy NGC 1407.
o	Table 1: <[CBS2007] NN> N=21 among (Nos 1-33).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBS2009]
[CBS2009]	(Clarke+Blanton+Sarazin+, 2009) (Not yet in Simbad)
Write:	<<[CBS2009] A>>
N:	7
Object:	Bubble (SIMBAD class: PartofG = Part of a Galaxy)
Note:	VLA and Chandra observations of the core of Abell 262.
in source:	B2 0149+35
Ref:	=2009ApJ...697.1481C
by	CLARKE T.E. , BLANTON E.L., SARAZIN C.L., ANDERSON L.D., GOPAL-KRISHNA, DOUGLASS E.M., KASSIM N.E.
	Astrophys. J., 697, 1481-1492 (2009)
	Tracing multiple generations of active galactic nucleus feedback in the core of Abell 262.
o	Fig. 7, Table 3: <[CBS2009] A> (Nos A-G).
o	B2 1049+35 and B2 0149+32 are misprints for B2 0149+35.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBS2011]
[CBS2011]	(Crighton+Bielby+Shanks+, 2011)
Write:	<<[CBS2011] QHHMMSS.ss+DDMMSS.s>> <<[CBS2011] NNN>>
N:	182+176
Object:	QSO + Absorber (SIMBAD class: Unknown = Object of Unknown Nature)
Stat.	in SIMBAD: Table C1 is completely incorporated.
Note:	AAT AAOmega spectroscopic observations of quasars and CIV absorption systems.
Ref:	=2011MNRAS.414...28C
by	CRIGHTON N.H.M. , BIELBY R., SHANKS T., INFANTE L., BORNANCINI C.G., BOUCHE N., LAMBAS D.G., LOWENTHAL J.D., MINNITI D., MORRIS S.L., PADILLA N., PEROUX C., PETITJEAN P., THEUNS T., TUMMUANGPAK P., WEILBACHER P.M., WISOTZKI L., WORSECK G.
	Mon. Not. R. Astron. Soc., 414, 28-49 (2011)
	The VLT LBG redshift survey– II. Interactions between galaxies and the IGM at z~ 3.
o	Table C1: <[CBS2011] QHHMMSS.ss+DDMMSS.s> N=182. Table C3: <[CBS2011] NNN> (Nos 1-176).
=E=	Catalogue in electronic form as <J/MNRAS/414/28/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBS2013]
[CBS2013]	(Carretti+Brown+Staveley-Smith+, 2013)
Write:	<<[CBS2013] NN>>
N:	13
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA 2.3GHz and Parkes 3.3GHz observations of N=13 compact sources in the galaxy cluster Abell 3667. Use of Parkes S-band Polarisation All Sky Survey (S-PASS) data.
in source:	ACO 3667
Ref:	=2013MNRAS.430.1414C
by	CARRETTI E. , BROWN S., STAVELEY-SMITH L., MALARECKI J.M., BERNARDI G., GAENSLER B.M., HAVERKORN M., KESTEVEN M.J., POPPI S.
	Mon. Not. R. Astron. Soc., 430, 1414-1422 (2013)
	Detection of a radio bridge in Abell 3667.
o	Table 1: <[CBS2013] NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBS2017]
[CBS2017]	(Chaves-Montero+Bonoli+Salvato+, 2017)
Write:	<<[CBS2017] ALH2LNNN>> <<[CBS2017] ALH3LNNN>>
N:	585+494
Object:	Poss. AGN (SIMBAD class: AGN_Candidate = Active Galaxy Nucleus Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=585+494 AGN candidates in ALHMAMBRA data, using the two- and three-line modes (2L and 3L in the formats) of the Emission Line Detector of Astrophysical Radiators (ELDAR) algorithm.
Ref:	=2017MNRAS.472.2085C
by	CHAVES-MONTERO J. , BONOLI S., SALVATO M., GREISEL N., DIAZ-GARCIA L.A., LOPEZ-SANJUAN C., VIIRONEN K., FERNANDEZ-SOTO A., POVIC M., ASCASO B., ARNALTE-MUR P., MASEGOSA J., MATUTE I., MARQUEZ I., CENARRO A.J., ABRAMO L.R., EDEROCLITE A., ALFARO E.J., MARIN-FRANCH A., VARELA J., CRISTOBAL-HORNILLOS D.
	Mon. Not. R. Astron. Soc., 472, 2085-2106 (2017)
	ELDAR, a new method to identify AGN in multi-filter surveys: the ALHAMBRA test case.
o	alh21.dat: <[CBS2017] ALH2LNNN> (Nos ALH2L000-ALH2L584). alh31.dat: <[CBS2017] ALH3LNNN> (Nos ALH3L000-ALH3L493).
=E=	Catalogue in electronic form as <J/MNRAS/472/2085/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBS82]
[CBS82]	(Cohen+Bieging+Schwartz, 1982)
Write:	<<[CBS82] HHMMSS.sss+DDMMSS.ss>>
N:	6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=6 VLA sources associated with 6 pre-main-sequence stars.
Ref:	=1982ApJ...253..707C
by	COHEN M. , BIEGING J.H., SCHWARTZ P.R.
	Astrophys. J., 253, 707-715 (1982)
	VLA observations of mass loss from T Tauri stars.
o	Table 1: <[CBS82] HHMMSS.sss+DDMMSS.ss> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBS97]
[CBS97]	(Cernis+Bartasiute+Straizys+, 1997)
Write:	<<[CBS97] NGC NNNN NN>> <<[CBS97] alf Vul N>> <<[CBS97] Pal 11 NN>> <<[CBS97] SA 64A N>> <<[CBS97] 22 Vul N>> <<[CBS97] Veil N>>
N:	72
Object:	* (SIMBAD class: Star)
Note:	N=72 stars in 11 fields. Field NGC 6535 is designated as field Ser I in 2002BaltA..11..417S. See also [SBC2002].
Ref:	=1997BaltA...6..573C
by	CERNIS K. , BARTASIUTE S., STRAIZYS V., JANULIS R.
	Baltic Astronomy, 6, 573-584 (1997)
	Standard stars for CCD photometry in the Vilnius system.
o	Table 2: <[CBS97] NGC 6535 NN> (Nos 1-11), <[CBS97] NGC 6760 N> (Nos 1-6), <[CBS97] NGC 6791 N> (Nos 1-5), <[CBS97] NGC 6802 N> (Nos 1-7), <[CBS97] alf Vul N> (Nos 1-5), <[CBS97] NGC 6819 N> (Nos 1-5), <[CBS97] Pal 11 NN> (Nos 1-12), <[CBS97] SA 64A N> (Nos 1-6), <[CBS97] SA 64B N> (Nos 1-5), <[CBS97] 22 Vul N> (Nos 1-5), <[CBS97] Veil N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBS98]
[CBS98]	(Couch+Barger+Smail+, 1998)= (HST)
Write:	<<[CBS98] AC 103 NNNN>> <<[CBS98] AC 118 NNNN>> <<[CBS98] AC 114 N.NNNN>>
N:	738
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies) ABELL 2744:[CN84] NNN, ABELL S0910:[CN84] NNN, ABELL S1077:[CN84] NNN
Note:	HST WFPC2 observations of 3 ClG.
in source:	ACCG 103 = ACO S 910
in source:	ACCG 118 = ACO 2744
in source:	ACCG 114 = ACO S 1077
Ref:	=1998ApJ...497..188C
by	COUCH W.J. , BARGER A.J., SMAIL I., ELLIS R.S., SHARPLES R.M.
	Astrophys. J., 497, 188-211 (1998)
	Morphological studies of the galaxy populations in distant ``Butcher-Oemler'' clusters with the Hubble Space Telescope. II. AC 103, AC 118, and AC 114 at z = 0.31.
o	cross-id. 'CN ACNNN NNNA' and B96 = '[BAE96] AC NNN NNN'
o	Table 4: <[CBS98] AC 103 NNNN> N=122 among (Nos 10-2013), <[CBS98] AC 118 NNNN> N=131 among (Nos 21-2006), <[CBS98] AC 114 N.NNNN> N=485.
=E=	Catalogue in electronic form as J/ApJ/497/188
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CBSS
CBSS	(Cappellaro+Benetti+Sabbadin+Salvatori+)
Write:	<<CBSS N>>
N:	3
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	See also HHG.
Ref:	=1994MNRAS.267..871C
by	CAPPELLARO E. , BENETTI S., SABBADIN F., SALVADORI L., TURATTO M., ZANIN C.
	Mon. Not. R. Astron. Soc., 267, 871-880 (1994)
	New emission nebulae in the POSS field 18h 48m +0°.
o	Table 1: <HHG LLL.l+BB.b> N=1, <CBSS N> (Nos 1-3).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CBV2001]
[CBV2001]	(Cecil+Bland-Hawthorn+Veilleux+, 2001) (Not yet in Simbad)
Write:	<<[CBV2001] NNN>>
N:	233
Object:	Filament (SIMBAD class: PartofG = Part of a Galaxy)
Note:	HST EFPC2 images of the edge-on galaxy NGC 3079. N=233 superbubble ionized filaments.
in source:	NGC 3079
Ref:	=2001ApJ...555..338C
by	CECIL G. , BLAND-HAWTHORN J., VEILLEUX S., FILIPPENKO A.V.
	Astrophys. J., 555, 338-355 (2001)
	Jet- and wind-driven ionized outflows in the superbubble and star-forming disk of NGC 3079.
o	Introduction: The most luminous known H2O maser = [CPF88] 095835.0+555517.6 in SIMBAD.
o	Fig.7, Table 3: <[CBV2001] NNN> (Nos 1-233).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBV2003]
[CBV2003]	(Carraro+Baume+Villanova, 2003)
Write:	<<[CBV2003] NGC 1883 NNN>>
N:	692
Object:	* (SIMBAD class: Star)
Note:	1.82m Copernico telescope AFOSC BVI CCD photometry of the open cluster NGC 1883.
in source:	NGC 1883
Ref:	=2003MNRAS.343..547C
by	CARRARO G. , BAUME G., VILLANOVA S.
	Mon. Not. R. Astron. Soc., 343, 547-551 (2003)
	NGC 1883: a neglected intermediate-age open cluster located in the outskirts of the Galactic disc.
o	<[CBV2003] NGC 1883 NNN> (Nos 1-692).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBW2001]
[CBW2001]	(Chengalur+Braun+Wieringa, 2001)
Write:	<<[CBW2001] JHHMM+DD.d>>
N:	2
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
in source:	ACO 3128
Ref:	=2001A&A...372..768C
by	CHENGALUR J.N. , BRAUN R., WIERINGA M.
	Astron. Astrophys., 372, 768-774 (2001)
	HI in Abell 3128.
o	Table 2: <[CBW2001] JHHMM+DD.d> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBW2017]
[CBW2017]	(Csengeri+Bontemps+Wyrowski+, 2017)
Write:	<<[CBW2017] GLLL.llll+BB.bbbb-MMN>> <<[CBW2017] LLL.llll+B.bbbb-MMN>> (not recognised by Simbad, but found in literature)
N:	100
Object:	Clump (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 7 Cycle 2 observations of N=100 sources in 35 infrared-quiet massive clumps selected from the ATLASGAL survey.
Ref:	=2017A&A...600L..10C
by	CSENGERI T. , BONTEMPS S., WYROWSKI F., MOTTE F., MENTEN K.M., BEUTHER H., BRONFMAN L., COMMERCON B., CHAPILLON E., DUARTE-CABRAL A., FULLER G.A., HENNING T., LEURINI S., LONGMORE S., PALAU A., PERETTO N., SCHULLER F., TAN J.C., TESTI L., TRAFICANTE A., URQUHART J.S.
	Astron. Astrophys., 600L, 10-10 (2017)
	ALMA survey of massive cluster progenitors from ATLASGAL. Limited fragmentation at the early evolutionary stage of massive clumps.
o	Fig. A.1, Table A.1: <[CBW2017] GLLL.llll+BB.bbbb-MMN> N=100.
=E=	Catalogue in electronic form as <J/A+A/600/L10/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBW93]
[CBW93]	(Colless+Burstein+Wegner+, 1993)
*****	Avoid the usage of [CBW93], prefer GIN
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBW93]
[CBW93]	(Collesss+Burstein+Wegner+, 1993)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBW96]
[CBW96]	(Clocchiatti+Benetti+Wheeler+, 1996)
Write:	<<[CBW96] A>> <<[CBW96] NN>>
N:	6+10
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Photometric sequence around the galaxy NGC 5377.
Ref:	=1996AJ....111.1286C
by	CLOCCHIATTI A. , BENETTI S., WHEELER J.C., WREN W., BOISSEAU J., CAPPELLARO E., TURATTO M., PATAT F., SWARTZ D.A., HARKNESS R.P., BROTHERTON M.S., WILLS B., HEMENWAY P., CORNELL M., FRUEH M., KAISER M.B.
	Astron. J., 111, 1286-1303 (1996)
	A study of SN 1992H in NGC 5377.
o	Table 1: <[CBW96] A> (Nos A-F), <[CBW96] NN> (Nos 1-10)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CBZ2015]
[CBZ2015]	(Coe+Bradley+Zitrin, 2015)
Write:	<<[CBZ2015] FFAN-SSss-MSSs>>
N:	7+5+13
Object:	Grav. lensed image of a G (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFC3 observations of N=7+5+13 high-redshift candidate galaxies in the fields of ACO 2744 and MCS J0416.1-2403, as part of the Hubble and Spitzer "Frontier Fields" program. The format encodes the field name FFAN (where A stands for C=Cluster or B = "Blank" parallel field) followed by the last four digits of right ascension and declination SSss-MSSs (the complete 2000 coordinate format being 00 14 SS.ss -30 2M SS.s in ACO 2744, 04 16 SS.ss -24 0M SS.s in MCS J0416.1-2403).
in source:	ACO 2744
in source:	MCS J0416.1-2403
Ref:	=2015ApJ...800...84C
by	COE D. , BRADLEY L., ZITRIN A.
	Astrophys. J., 800, 84 (2015)
	Frontier Fields: high-redshift predictions and early results.
o	Tables 4-6: <[CBZ2015] FFAN-SSss-MSSs> N=7+5+13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CC
CC	(Courtes+Cruvellier)
*****	Avoid the usage of CC, prefer [CC65]
Origin	of the Acronym: L (1975ApJ...199..591S)
Details on Acronym: CC
CC	(Cincinnati obs.)
*****	Avoid the usage of CC, prefer Ci
Details on Acronym: CC
CC	(Cluster Candidate)
*****	Avoid the usage of CC, prefer [IBP2002]
Origin	of the Acronym: L (2005A&A...435..107I)
Details on Acronym: [CC2000]
[CC2000]	(Combes+Charmandaris, 2000)
Write:	<<[CC2000] HHMM+DDd>>
N:	1
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	A new QSO is found: 1923+210.
Ref:	=2000A&A...357...75C
by	COMBES F. , CHARMANDARIS V.
	Astron. Astrophys., 357, 75-83 (2000)
	Search for molecular gas in HVCs by HCO^+ absorption.
o	Table 1: <[CC2000] HHMM+DDd> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CC2002]
[CC2002]	(Cedres+Cepa, 2002)
Write:	<<[CC2002] NGC 5457 NNN>> <<[CC2002] NGC 4395 NNN>>
N:	338+158
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	NOT observations.
in source:	NGC 5457 = M 101
in source:	NGC 4395
Ref:	=2002A&A...391..809C
by	CEDRES B. , CEPA J.
	Astron. Astrophys., 391, 809-821 (2002)
	Distributions, equivalent widths and metallicities of the H II regions in the spiral galaxies NGC 5457 and NGC 4395.
o	Table 3: <[CC2002] NGC 5457 NNN> (Nos 1-338). Table 6: <[CC2002] NGC 4395 NNN> (Nos 1-158).
=E=	Catalogue in electronic form as J/A+A/391/809
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CC2004]
[CC2004]	(Clark+Crowther, 2004)= ([CC2004a])
Write:	<<[CC2004] JHHMMSS.s+DDMMSS.s>>
N:	2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of the galaxy IC 10: position for the bright X-ray source [BWF97] IC 10 X-1. Two new possible counterparts to the X-ray source are found.
in source:	IC 10
Ref:	=2004A&A...414L..45C
by	CLARK J.S. , CROWTHER P.A.
	Astron. Astrophys., 414, 45-48 (2004)
	On the Wolf-Rayet counterpart to IC 10 X-1.
o	Table 1: <[CC2004] JHHMMSS.s+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CC2004a]
[CC2004a]	(Clark+Crowther, 2004)
*****	Avoid the usage of [CC2004a], prefer [CC2004]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CC2004b]
[CC2004b]	(Chapuis+Corbel, 2004)
Write:	<<[CC2004b] GRS 1915+105 MC VV>>
N:	7
Object:	Absorber
Note:	IRAM and SEST observations. N=7 molecular clouds identified in the spectrum of Granat 1915+105. The 'MC' are in the line of sight of Granat 1915+105, and in the format 'VV' is the rounded LSR velocity.
Ref:	=2004A&A...414..659C
by	CHAPUIS C. , CORBEL S.
	Astron. Astrophys., 414, 659-665 (2004)
	On the optical extinction and distance of GRS 1915+105.
o	Table 1: <[CC2004b] GRS 1915+105 MC VV> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CC2009]
[CC2009]	(Carraro+Costa, 2009)
Write:	<<[CC2009] NNNN>>
N:	7425
Object:	* (SIMBAD class: Star)
Note:	CTIO 1.0m telescope photometry of the star cluster Shorlin 1.
in source:	NAME Shorlin 1
Ref:	=2009A&A...493...71C
by	CARRARO G. , COSTA E.
	Astron. Astrophys., 493, 71-78 (2009)
	Searching for spiral features in the outer Galactic disk. The field towards WR38 and WR38a.
o	Catalog: <[CC2009] NNNN> (Nos 1-7425).
=E=	Catalogue in electronic form as J/A+A/493/71
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CC2011]
[CC2011]	(Cohen+Clarke, 2011)
Write:	<<[CC2011] A>>
N:	9
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA observations at 1425, 325 and 74MHz of N=9 radio sources in the galaxy cluster ACO 2443.
in source:	ACO 2443
Ref:	=2011AJ....141..149C
by	COHEN A.S. , CLARKE T.E.
	Astron. J., 141, 149 (2011)
	An ultra-steep-spectrum radio relic in the galaxy cluster A2443.
o	Figs 1-8: <[CC2011] A> (Nos A-I).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CC2015]
[CC2015]	(Chiang+Chen, 2015)
Write:	<<[CC2015] Oph JHHMMSS+DDMMSS>>
N:	3
Object:	T dwarf * + L dwarf * (SIMBAD class: BrownD* = Brown Dwarf)
Stat:	is completely incorporated in Simbad
Note:	Gemini South FLAMINGOS-2 spectroscopy of N=2 T dwarfs and N=1 L dwarf in the dark cloud LDN 1688.
in source:	NAME RHO OPH CLOUD:LDN 1688 = LDN 1688
Ref:	=2015ApJ...811L..16C
by	CHIANG P. , CHEN W.P.
	Astrophys. J., 811L, 16 (2015)
	Discovery of young methane dwarfs in the ρ Ophiuchi L 1688 dark cloud.
o	<[CC2015] Oph JHHMMSS+DDMMSS> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CC65]
[CC65]	(Courtes+Cruvellier, 1965)= (CC)
Write:	<<[CC65] NNN>>
N:	101
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Finding chart. Superseded by BCLMP
in source:	M 33 = NGC 598
Ref:	=1965AnAp...28..683C
by	COURTES G. , CRUVELLIER P.
	Ann. Astrophys., 28, 683-690 (1965)
	Etudes des galaxies en lumiere monochromatique H-α. I. Messier 33 (NGC 598).
o	<[CC65] NNN> N=101, Superseded by [BCL74], Use [BCL74]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CC74]
[CC74]	(Clark+Crawford, 1974)
Write:	<<[CC74] HHMMSS.s+DDMMSS>>
N:	513
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	The authors don't give any format to their list, so we use the coordinates as format.
Ref:	=1974AuJPh..27..713C
by	CLARK D.H. , CRAWFORD D.F.
	Australian J. Phys., 27, 713-727 (1974)
	A catalogue of small-diameter radio sources close to the galactic plane.
o	<[CC74] HHMMSS.s+DDMMSS> N=513
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CC87]
[CC87]	(Cowley+Crampton, 1987)
Write:	<<[CC87] HHMM.m+DDMM>> <<[CC87] HHMM.m+DDd>>
N:	15
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Note:	See also [CR82], [CP83], [CSC85], [CCH87], [CCS88], [CCH90], [CCH91], and [CCH92]
Ref:	=1987AJ.....94...16C
by	COWLEY A.P. , CRAMPTON D.
	Astron. J., 94, 16-22 (1987)
	Broad-absorption-line quasar candidates discovered in the CFHT/MMT QSO survey.
o	Table I: <[CC87] HHMM.m+DDMM>, <[CC87] HHMM.m+DDd>, N=15
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CC91]
[CC91]	(Clowes+Campusano, 1991)
Write:	<<[CC91] HHMMSS.s+DDMMSS>>
N:	118
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Ref:	=1991MNRAS.249..218C
by	CLOWES R.G. , CAMPUSANO L.E.
	Mon. Not. R. Astron. Soc., 249, 218-226 (1991)
	A 100-200 Mpc group of quasars.
o	Tables 1, 2: <[CC91] HHMMSS.s+DDMMSS> N=83
Ref:	=1999MNRAS.309...48C
by	CLOWES R.G. , CAMPUSANO L.E., GRAHAM M.J.
	Mon. Not. R. Astron. Soc., 309, 48-62 (1999)
	Further observations of quasars in ESO/SERC field 927.
o	Table 2: <[CC91] HHMMSS.s+DDMMSS> N=59 new.
=E=	Catalogue in electronic form as J/MNRAS/249/218
=E=	Catalogue in electronic form as <J/MNRAS/309/48/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CC96]
[CC96]	(Clements+Couch, 1996)
Write:	<<[CC96] NAN>>
N:	8
Object:	Cand. primeval G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations. Candidate primeval galaxies in the Hubble Deep Field. In the format 'NAN', The first number stands for chip (Nos 2-4)
in source:	NAME HDFN
Ref:	=1996MNRAS.280L..43C
by	CLEMENTS D.L. , COUCH W.J.
	Mon. Not. R. Astron. Soc., 280, 43-47 (1996)
	Candidate primeval galaxies in the Hubble Deep Field.
o	Table 1: <[CC96] NAN> (Nos 2P1-2P4, 3P1-3P2, 4P1-4P2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CC98]
[CC98]	(Comeron+Claes, 1998)
Write:	<<[CC98] LI-LMC 1501 W>>
N:	2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	ISOCAM observations of the field of the source LI-LMC 1501 in the LMC. N=2 embedded stars are identified.
in source:	Magellanic Clouds:LMC:LI-LMC 1501 = LI-LMC 1501
Ref:	=1998A&A...335L..13C
by	COMERON F. , CLAES P.
	Astron. Astrophys., 335, 13-16 (1998)
	Compact HII regions in the Large Magellanic Cloud observed by ISO.
o	Table 2: <[CC98] LI-LMC 1501 W> (Nos E, W).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCA2015]
[CCA2015]	(Chiang+Chen+Albert+, 2015)
Write:	<<[CCA2015] NNa>>
N:	31
Object:	Poss. Brown Dwarf (SIMBAD class: BrownD*_Candidate = Brown Dwarf Candidate)
Note:	CFHT 3.6m WIRCam and Spitzer c2d mid-infrared observations of N=31 T dwarf candidates in the dark cloud LDN 1688.
in source:	NAME Oph Molecular Cloud
Ref:	=2015MNRAS.448..522C
by	CHIANG P. , CHEN W.-P., ALBERT L., LIU M., MAGNIER E.A.
	Mon. Not. R. Astron. Soc., 448, 522-540 (2015)
	Searching for T dwarfs in the ρ Oph dark cloud L 1688.
o	Table 3: <[CCA2015] NNa> (Nos 1-28, 17b, 20b, 22b).
o	In Figure 1, 2MASS J10595219+3041498 is a probable misprint for 2MASS J10595185+3042059.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCA99]
[CCA99]	(Cotton+Condon+Arbizzani, 1999)
Write:	<<[CCA99] UGC NNNNNa>> <<[CCA99] UGC NNNNNAa>>
N:	829
Object:	G (SIMBAD class: Galaxy)
Note:	This list concerns UGC galaxies which are splitted in different components. DSS positions of UGC galaxies.
Ref:	=1999ApJS..125..409C
by	COTTON W.D. , CONDON J.J., ARBIZZANI E.
	Astrophys. J., Suppl. Ser., 125, 409-412 (1999)
	Arcsecond positions of UGC galaxies.
o	Table 1: <[CCA99] UGC NNNNNa>, <[CCA99] UGC NNNNNAa>, N=829.
=E=	Catalogue in electronic form as J/ApJS/125/409
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CCABS
CCABS	(Catalog of Chromospherically Active Binary Stars)
Write:	<<CCABS NNN>>
N:	168
Object:	SB (SIMBAD class: SB* = Spectroscopic Binary)
Stat:	is completely incorporated in Simbad
Note:	Superseded by CABS (1993A&AS..100..173S) with a different numbering
Ref:	=1988A&AS...72..291S
by	STRASSMEIER K.G. , HALL D.S., ZEILIK M., NELSON E., EKER Z., FEKEL F.C.
	Astron. Astrophys., Suppl. Ser., 72, 291-345 (1988)
	A catalog of chromospherically active binary stars.
o	More recent version in 1993A&AS..100..173S (CDS Catalog V/76)
o	Table I: <CCABS NNN> (Nos 1-168)
=E=	Catalogue in electronic form as V/71
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CCAC
CCAC	(Carte du Ciel and Astrographic Catalogue)
Write:	<<CCAC NNNN>>
N:	9055
Object:	* (SIMBAD class: Star)
Note:	Use of astrometric data from four Carte du Ciel (CdC) and one Astrographic Catalogue (AC) plates of the Cordoba Astronomical Observatory collection (Argentina) in the region of the open cluster Collinder 132.
in source:	Cl Collinder 132
Ref:	=2010A&A...521A..39O
by	ORELLANA R.B. , DE BIASI M.S., BUSTOS FIERRO I.H., CALDERON J.H.
	Astron. Astrophys., 521A, 39-39 (2010)
	A revisit to the region of Collinder 132 using Carte du Ciel and Astrographic Catalogue plates.
o	(Erratum) + corrigendum vol. 534 p. C1 (2011)
o	Table ccac.dat: <CCAC NNNN> (Nos 1-9055).
=E=	Catalogue in electronic form as J/A+A/521/A39
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CCB2009]
[CCB2009]	(Casey+Chapman+Beswick+, 2009)
Write:	<<[CCB2009] RG JHHMMSS.ss+DDMMSS.s>>
N:	8
Object:	rG (SIMBAD class: RadioG = Radio Galaxy)
Note:	N=8 submm-faint radio galaxies detected at 70mum by Spitzer.
Ref:	=2009MNRAS.399..121C
by	CASEY C.M. , CHAPMAN S.C., BESWICK R.J., BIGGS A.D., BLAIN A.W., HAINLINE L.J., IVISON R.J., MUXLOW T.W.B., SMAIL I.
	Mon. Not. R. Astron. Soc., 399, 121-128 (2009)
	Confirming a population of hot-dust dominated, star-forming, ultraluminous galaxies at high redshift.
o	Table 1: <[CCB2009] RG JHHMMSS.ss+DDMMSS.s> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCB2012]
[CCB2012]	(Cedres+Cepa+Bongiovanni+, 2012)
Write:	<<[CCB2012] NGC628 NNN>> <<[CCB2012] NGC6946 NNN>>
N:	435 (SIMBAD class: HIIReg = HII Region)
Note:	NOT ALFOSC observations of NGC 628 and NGC 6946.
in source:	NGC 628
in source:	NGC 6946
Ref:	=2012A&A...545A..43C
by	CEDRES B. , CEPA J., BONGIOVANNI A., CASTANEDA H., SANCHEZ-PORTAL M., TOMITA A.
	Astron. Astrophys., 545A, 43-43 (2012)
	Two-dimensional metallicity distribution of the ionized gas in NGC 628 and NGC 6946.
o	<[CCB2012] NGC628 NNN>,<[CCB2012] NGC6946 NNN> N=435
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCB99]
[CCB99]	(Chereul+Creze+Bienayme, 1999)
Write:	<<[CCB99] NN>> <<[CCB99] Pegasus N>>
N:	17+2
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Ref:	=1999A&AS..135....5C
by	CHEREUL E. , CREZE M., BIENAYME O.
	Astron. Astrophys., Suppl. Ser., 135, 5-28 (1999)
	The distribution of nearby stars in phase space mapped by Hipparcos. III. Clustering and streaming among A-F type stars.
o	Table 1: <[CCB99] NN> (Nos 1-17), <[CCB99] Pegasus N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CCC
CCC	(Centaurus Cluster Catalogue)
Write:	<<CCC NNN>>
N:	296
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	Centaurus Cluster = ACO 3526
Ref:	=1997A&AS..124....1J
by	JERJEN H. , DRESSLER A.
	Astron. Astrophys., Suppl. Ser., 124, 1-12 (1997)
	Studies of the Centaurus cluster. I. A catalogue of galaxies in the central region of the Centaurus cluster.
o	<CCC NNN> (Nos 1-296)
=E=	Catalogue in electronic form as J/A+AS/124/1
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CCC
CCC	(Coma Cluster Catalogue)
*****	Avoid the usage of CCC, prefer ComaCC
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CCC2007]
[CCC2007]	(Chilingarian+Cayatte+Chemin+, 2007)
Write:	<<[CCC2007] ACO496JHHMMSS.ss+DDMMSS.s>> <<[CCC2007] A496cE>> <<[CCC2007] A496gN>>
N:	3
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	ESO-VLT FLAMES-Giraffe spectrograph observations of ACO 496.
in source:	ACO 496
Ref:	=2007A&A...466L..21C
by	CHILINGARIAN I. , CAYATTE V., CHEMIN L., DURRET F., LAGANA T.F., ADAMI C., SLEZAK E.
	Astron. Astrophys., 466L, 21-24 (2007)
	Discovery of a new M 32-like ``Compact Elliptical'' galaxy in the halo of the Abell 496 cD galaxy.
o	Text, Table 2: <[CCC2007] ACO496JHHMMSS.ss+DDMMSS.s> N=3, <[CCC2007] A496cE> N=1, <[CCC2007] A496gN> (Nos g1, g2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCC2011]
[CCC2011]	(Chapin+Chapman+Coppin+, 2011)
Write:	<<[CCC2011] SID250 NNN>> <<[CCC2011] SID350 NNN>> <<[CCC2011] SID500 NNN>> <<[CCC2011] SID870 NNN>> <<[CCC2011] NNN>>
N:	389+362+267+122+118
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	Use of BLAST and LESS data in the Extended Chandra Deep Field-South.
in source:	NAME ECDFS
Ref:	=2011MNRAS.411..505C
by	CHAPIN E.L. , CHAPMAN S.C., COPPIN K.E., DEVLIN M.J., DUNLOP J.S., GREVE T.R., HALPERN M., HASSELFIELD M.F., HUGHES D.H., IVISON R.J., MARSDEN G., MONCELSI L., NETTERFIELD C.B., PASCALE E., SCOTT D., SMAIL I., VIERO M., WALTER F., WEISS A., VAN DER WERF P.
	Mon. Not. R. Astron. Soc., 411, 505-549 (2011)
	A joint analysis of BLAST 250–500 µm and LABOCA 870 µm observations in the Extended Chandra Deep Field-South.
o	Table C1: <[CCC2011] SID250 NNN> (Nos 1-389). Table C2: <[CCC2011] SID350 NNN> (Nos 1-362). Table C3: <[CCC2011] SID500 NNN> (Nos 5-267). Table C4: <[CCC2011] SID870 NNN> (Nos 1-122). Table C5: <[CCC2011] NNN> (Nos 1-118).
=E=	Catalogue in electronic form as <J/MNRAS/411/505/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCC2012]
[CCC2012]	(Clementini+Cignoni+Contreras Ramos+, 2012)
Write:	<<[CCC2012] VNN>>
N:	14 (SIMBAD class: Variable* = Variable Star)
Note:	Search for variable stars in archival HST WFPC2 observations of the ultra-faint dwarf galaxy Leo T.
in source:	NAME Leo T dSph
Ref:	=2012ApJ...756..108C
by	CLEMENTINI G. , CIGNONI M., CONTRERAS RAMOS R., FEDERICI L., RIPEPI V., MARCONI M., TOSI M., MUSELLA I.
	Astrophys. J., 756, 108 (2012)
	Variability and star formation in Leo T, the lowest luminosity star-forming galaxy known today.
o	Table 2: <[CCC2012] VNN> (Nos V1-V14)
=E=	Catalogue in electronic form as <J/ApJ/756/108/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCC2013]
[CCC2013]	(Casey+Chen+Cowie+, 2014)= (SMM)
Write:	<<[CCC2013] SMM JHHMMSS.s+DDMMSS>> <<[CCC2013] {450\|850}.NNN>> <<[CCC2013] {450\|850}.NNN N>>
N:	102+123+?
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	JCMT SCUBA-2 450µm and 850µm observations of the COSMOS field.
in source:	NAME COSMOS Field
Ref:	=2013MNRAS.436.1919C
by	CASEY C.M. , CHEN C.-C., COWIE L.L., BARGER A.J., CAPAK P., ILBERT O., KOSS M., LEE N., LE FLOC'H E., SANDERS D.B., WILLIAMS J.P.
	Mon. Not. R. Astron. Soc., 436, 1919-1954 (2013)
	Characterization of Scuba-2 450µm and 850µm selected galaxies in the COSMOS field.
o	Table 1, col(1): <[CCC2013] SMM JHHMMSS.s+DDMMSS> N=78 = Table 1, col(2): <[CCC2013] 450.NN> (Nos 450.00-450.77). Table 2, col(1): <[CCC2013] SMM JHHMMSS.s+DDMMSS> N=99 = Table 2, col(2): <[CCC2013] 850.NN> (Nos 850.00-850.98). Table 5: <[CCC2013] 450.NN N> N=?. Table 7: <[CCC2013] 850.NN N> N=?. Table 4, col(1): <[CCC2013] SMM JHHMMSS.s+DDMMSS> N=24, Table 4, col(2): <[CCC2013] 850.NNN> N=24 among (Nos 850.09-850.163), Table 4, col(3): <[CCC2013] 450.NNN> N=24 among (Nos 450.78-450.252). Table 6: <[CCC2013] 450.NNN N> N=66, <[CCC2013] 850.NNN N> N=66.
=E=	Catalogue in electronic form as <J/MNRAS/436/1919/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCC2015]
[CCC2015]	(Casey+Cooray+Capak+, 2015)
Write:	<<[CCC2015] PCL1002>> <<[CCC2015] LBG JHHMMSS.ss+DDMMSS.s>> <<[CCC2015] DSFG JHHMMSS.ss+DDMMSS.s>>
N:	7+34+1
Object:	Protocluster + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Keck MOSFIRE spectroscopic observations of N=6+34 galaxy members of a protocluster at z=2.47 in the COSMOS field.
in source:	NAME COSMOS Field
Ref:	=2015ApJ...808L..33C
by	CASEY C.M. , COORAY A., CAPAK P., FU H., KOVAC K., LILLY S., SANDERS D.B., SCOVILLE N.Z., TREISTER E.
	Astrophys. J., 808L, 33 (2015)
	A massive, distant proto-cluster at z = 2.47 caught in a phase of rapid formation?
o	Text: <[CCC2015] PCL1002> N=1. Table 2: <[CCC2015] LBG JHHMMSS.ss+DDMMSS.s> N=34, <[CCC2015] DSFG JHHMMSS.ss+DDMMSS.s> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCC2018]
[CCC2018]	(Carballo-Bello+Corral-Santana+Catelan+, 2020)
Write:	<<[CCC2018] NGC 7492 NN>>
N:	71
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT VIMOS spectroscopy of N=71 stars around the globular cluster NGC 7492.
in source:	NGC 7492
Ref:	=2018MNRAS.474.4766C
by	CARBALLO-BELLO J.A. , CORRAL-SANTANA J.M., CATELAN M., MARTINEZ-DELGADO D., MUNOZ R.R., SOLLIMA A., NAVARRETE C., DUFFAU S., COTE P., MORA M.D.
	Mon. Not. R. Astron. Soc., 474, 4766-4771 (2018)
	The globular cluster NGC 7492 and the Sagittarius tidal stream: together but unmixed.
o	Table 1: <[CCC2018] NGC 7492 NN> (Nos 1-71).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CCCGS
CCCGS	(Catalog of Cool Carbon Gal. *)
**	catalog: use CGCS
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CCCS
CCCS	(Catalog of Cool Carbon *)
**	catalog: use C*
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CCD
CCD	(CCD image source)
*****	Avoid the usage of CCD, prefer [SSJ82]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CCD2001]
[CCD2001]	(Christian+Craig+Dupuis+, 2001)
Write:	<<[CCD2001] EUVE J1952+47.8 N>>
N:	2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	EUVE optical identification of previously unidentified sources. N=2 possible identifications for EUVE J1952+47.8.
Ref:	=2001AJ....122..378C
by	CHRISTIAN D.J. , CRAIG N., DUPUIS J., ROBERTS B.A., MALINA R.F.
	Astron. J., 122, 378-391 (2001)
	Extreme ultraviolet explorer optical identification campaign. IV. A northern hemisphere sample of active late-type stars and typical EUV sources.
o	Table 2: <[CCD2001] EUVE J1952+47.8 N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCD2003]
[CCD2003]	(Chu+Chen+Danforth+, 2003)
Write:	<<[CCD2003] N30B-W>> <<[CCD2003] NN>>
N:	2+16
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 images of the HII region LHA 120-N 30B. LHA 120-N 30B has 2 HII lobes: 'N30B-E' and 'N30B-W'. N=16 stars (Nos 1-16) in the vicinity of LHA 120-N 30B.
in source:	Magellanic Clouds:LMC:LHA 120-N 30B = LHA 120-N 30B
Ref:	=2003AJ....125.2098C
by	CHU Y.-H. , CHEN C.-H.R., DANFORTH C., DUNNE B.C., GRUENDL R.A., NAZE Y., OEY M.S., POINTS S.D.
	Astron. J., 125, 2098-2107 (2003)
	The wind of the B[e] supergiant Henize S22 viewed through a reflection nebula in DEM L106.
o	Fig.1: <[CCD2003] N30B-W> (Nos N30B-E, N30B-W). Table 2: <[CCD2003] NN> (Nos 1-16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCD2006]
[CCD2006]	(Cohen+Chapman+Deacon+, 2006)
Write:	<<[CCD2006] A>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA observations of the PN G354.8-00.5 around V* V1018 Sco.
Ref:	=2006MNRAS.369..189C
by	COHEN M. , CHAPMAN J.M., DEACON R.M., SAULT R.J., PARKER Q.A., GREEN A.J.
	Mon. Not. R. Astron. Soc., 369, 189-196 (2006)
	Radio observations of the planetary nebula around the OH/IR star OH354.88-0.54 (V1018 Sco).
o	Table 2, Fig.1: <[CCD2006] A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCD2008]
[CCD2008]	(Chilingarian+Cayatte+Durret+, 2008)
Write:	<<[CCD2008] G-NN>> <<[CCD2008] G-AN>> <<[CCD2008] ACO 496 JHHMMSS.ss+DDMMSS.s>>
N:	48
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	CFHT and VLT FLAMES-Giraffe observations of early-type galaxies in ACO 496.
in source:	ACO 496
Ref:	=2008A&A...486...85C
by	CHILINGARIAN I.V. , CAYATTE V., DURRET F., ADAMI C., BALKOWSKI C., CHEMIN L., LAGANA T.F., PRUGNIEL P.
	Astron. Astrophys., 486, 85-97 (2008)
	Kinematics and stellar populations of low-luminosity early-type galaxies in the Abell 496 cluster.
o	Figs A1-A48, Table A1: <[CCD2008] G-NN> (Nos G-01 to G-46), <[CCD2008] G-AN> (Nos G-A1, G-A2) = <[CCD2008] ACO 496 JHHMMSS.ss+DDMMSS.s> N=48.
=E=	Catalogue in electronic form as J/A+A/486/85
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCD97]
[CCD97]	(Craig+Christian+Dupuis+, 1997)
Write:	<<[CCD97] EUVE JHHMM+DDd NA>>
N:	64
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=64 counterpart candidates for 27 EUVE Finding charts in Fig.1
Ref:	=1997AJ....114..244C
by	CRAIG N. , CHRISTIAN D.J., DUPUIS J., ROBERTS B.A.
	Astron. J., 114, 244-257 (1997)
	Extreme Ultraviolet Explorer optical identification campaign. III. A southern hemisphere sample of active late-type stars and white dwarfs.
o	Table 2: <[CCD97] EUVE JHHMM-DDd NA> N=64
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCD99]
[CCD99]	(Corbel+Chapuis+Dame+, 1999)= (MC)
Write:	<<[CCD99] MC -VVV>>
N:	8
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	ESO SEST observations. N=8 molecular clouds along the line of sight to 'NAME SGR 1627-41'. In the format '-VVV' stands for the radial velocity.
Ref:	=1999ApJ...526L..29C
by	CORBEL S. , CHAPUIS C., DAME T.M., DUROUCHOUX P.
	Astrophys. J., 526, 29-32 (1999)
	The distance to the soft γ repeater Sgr 1627-41.
o	Table 1: <[CCD99] MC -VVV> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CCDM
CCDM	(Catalog of Comp. of Double and Mult. *)
Write:	<<CCDM JHHMMm+DDMMAAA>>
N:	74861
Object:	(SIMBAD class: = Double or Multiple Star)
Ref:	=1983BICDS..24...83D
by	DOMMANGET J.
	Bull. Inf. Centre Donnees Stellaires, 24, 83-90 (1983)
	Un catalogue des composantes d'etoiles doubles et multiples (C.C.D.M.).
o	<CCDM JHHMMm+DDMMA> N=74861.
Ref:	=1994CoORB.115....1D
by	DOMMANGET J. , NYS O.
	Com. de l'Observ. Royal de Belgique, 115, 1-None (1994)
	Catalogue des composantes d'etoiles doubles et multiples (CCDM) premiere edition - Catalogue of the components of double and multiple stars (CCDM) first edition.
o	<CCDM JHHMMm+DDMMA> N=74861.
=E=	Catalogue in electronic form as I/274
Details on Acronym: CCE
CCE	(Cambresy+Copet+Epchtein+)
*****	Avoid the usage of CCE, prefer [CCE98]
Origin	of the Acronym: L (2007A&A...461..669R)
Details on Acronym: [CCE2018]
[CCE2018]	(Castro+Crowther+Evans+, 2018)
Write:	<<[CCE2018] NNNN>>
N:	2255
Object:	* (SIMBAD class: Star)
Note:	VLT MUSE spectroscopic observations of N=2253 stars in the Tarantula Nebula.
in source:	Magellanic Clouds:LMC:30 Dor Nebula = 30 Dor Nebula
Ref:	=2018A&A...614A.147C
by	CASTRO N. , CROWTHER P.A., EVANS C.J., MACKEY J., CASTRO-RODRIGUEZ N., VINK J.S., MELNICK J., SELMAN F.
	Astron. Astrophys., 614A, 147-147 (2018)
	Mapping the core of the Tarantula Nebula with VLT-MUSE. I. Spectral and nebular content around R136.
o	Table 3: <[CCE2018] NNNN> N=2255 among (Nos 13-3204).
=E=	Catalogue in electronic form as J/A+A/614/A147
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCE98]
[CCE98]	(Cambresy+Copet+Epchtein+, 1998)= (Cam) = (CCE) = ([CCE98a])
Write:	<<[CCE98] 1-NNN>> <<[CCE98] 2-NN>>
N:	126+54
Object:	Poss. YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=126 known TTau*, format '1-NNN'. Table 2: N=54 YSO candidates discovered by DENIS, format '2-NN'.
in source:	NAME Cha I
Ref:	=1998A&A...338..977C
by	CAMBRESY L. , COPET E., EPCHTEIN N., DE BATZ B., BORSENBERGER J., FOUQUE P., KIMESWENGER S., TIPHENE D.
	Astron. Astrophys., 338, 977-987 (1998)
	New young stellar object candidates in the Chamaeleon I molecular cloud discovered by DENIS.
o	Table 1: <[CCE98] 1-NNN> (Nos 1-1 to 1-126). Table 2: <[CCE98] 2-NN> (Nos 2-1 to 2-54). Table 1: <Hn NNW> (Nos 10E, 10W, 12E, 12W, 21E, 21W) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCE98a]
[CCE98a]	(Cambresy+Copet+Epchtein+, 1998)
*****	Avoid the usage of [CCE98a], prefer [CCE98]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCE98b]
[CCE98b]	(Carey+Clark+Egan+, 1998)= (IRDC)
Write:	<<[CCE98b] LLL.ll+B.bb>>
N:	14
Object:	Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	H2CO observations with SPIRIT III on MSX satellite. IR Dark Clouds (IRDC) in the galactic plane survey. See also [CFR2000] and [PWC2006].
Ref:	=1998ApJ...508..721C
by	CAREY S.J. , CLARK F.O., EGAN M.P., PRICE S.D., SHIPMAN R.F., KUCHAR T.A.
	Astrophys. J., 508, 721-728 (1998)
	The physical properties of the midcourse space experiment galactic infrared-dark clouds.
o	Table 2: <[CCE98b] LLL.ll+B.bb> N=10
Ref:	=2000ApJ...543L.157C
by	CAREY S.J. , FELDMAN P.A., REDMAN R.O., EGAN M.P., MacLEOD J.M., PRICE S.D.
	Astrophys. J., 543, 157-161 (2000)
	Submillimeter observations of midcourse space experiment galactic infrared-dark clouds.
o	Text: <[CCE98b] LLL.ll+B.bb> N=4 added. Table 1, Fig.1: <[CFR2000] GLLL.ll+B.bb PN> N=11.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCF2011]
[CCF2011]	(Clementini+Contreras Ramos+Federici+, 2011)
Write:	<<[CCF2011] JHHMMSS.s+DDMMSS>> <<[CCF2011] VN>>
N:	274+6
Object:	Poss. V* + V* (SIMBAD class: Variable*_Candidate = Variable Star Candidate)
Note:	LBT LBC-blue BV photometry of N=274 candidate variable stars in two fields at the periphery of M 31.
in source:	M 31 = NGC 224
Ref:	=2011ApJ...743...19C
by	CLEMENTINI G. , CONTRERAS RAMOS R., FEDERICI L., MACARIO G., BECCARI G., TESTA V., CIGNONI M., MARCONI M., RIPEPI V., TOSI M., BELLAZZINI M., FUSI PECCI F., DIOLAITI E., CACCIARI C., MARANO B., GIALLONGO E., RAGAZZONI R., DI PAOLA A., GALLOZZI S., SMAREGLIA R.
	Astrophys. J., 743, 19 (2011)
	Hide and seek between Andromeda's halo, disk, and giant stream.
o	Table 9: <[CCF2011] JHHMMSS.s+DDMMSS> N=274. Table 10: <[CCF2011] VN> (Nos V1-V6).
=E=	Catalogue in electronic form as J/ApJ/743/19
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCF2016]
[CCF2016]	(Cappelluti+Comastri+Fontana+, 2016)
Write:	<<[CCF2016] NNN>>
N:	698
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	N=698 unique X-ray sources in the GOODS South field. Use of 4Ms Chandra Deep Field South (CDFS) and CANDELS GOODS-South H-band selected data.
in source:	NAME GOODS South Field
Ref:	=2016ApJ...823...95C
by	CAPPELLUTI N. , COMASTRI A., FONTANA A., ZAMORANI G., AMORIN R., CASTELLANO M., MERLIN E., SANTINI P., ELBAZ D., SCHREIBER C., SHU X., WANG T., DUNLOP J.S., BOURNE N., BRUCE V.A., BUITRAGO F., MICHALOWSKI M.J., DERRIERE S., FERGUSON H.C., FABER S.M., VITO F.
	Astrophys. J., 823, 95 (2016)
	Chandra counterparts of CANDELS GOODS-S sources.
o	catalog.dat: <[CCF2016] NNN> N=698 among (Nos 1-704).
=E=	Catalogue in electronic form as J/ApJ/823/95
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCF97]
[CCF97]	(Carignan+Cote+Freeman+, 1997)
Write:	<<[CCF97] GN>>
N:	9
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=9 satellites galaxies of NGC 5084
Ref:	=1997AJ....113.1585C
by	CARIGNAN C. , COTE S., FREEMAN K.C., QUINN P.J.
	Astron. J., 113, 1585-1590 (1997)
	NGC 5084: a massive disk galaxy accreting its satellites?
o	Table 1: <[CCF97] GN> (Nos G1-G9)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCF98]
[CCF98]	(Conner+Cooray+Flechter+, 1998)
Write:	<<[CCF98] A>> <<[CCF98] JHHMMSS.ss+DDMMSS.s>>
N:	3+3
Object:	Core (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Radio observations of MITG J0248+0641: N=1 central core 'A' and N=2 hotspots (Nos B-C). N=1 Optical Counterpart 'J024858.23+064143.3', and N=2 nearby sources, format 'JHHMMss.ss+DDMMSS.s'
in source:	MITG J0248+0641
Ref:	=1998AJ....115...37C
by	CONNER S.R. , COORAY A.R., FLETCHER A.B., BURKE B.F., LEHAR J., GARNAVICH P.M., MUXLOW T.W.B., THOMASSON P., BLAKESLEE J.P.
	Astron. J., 115, 37-48 (1998)
	Ringlike structure in the radio lobe of MG 0248+0641.
o	Fig.4: <[CCF98] A> (Nos A-C). p.38: <[CCF98] JHHMMSS.ss+DDMMSS.s> N=3
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCG2000]
[CCG2000]	(Carson+Cool+Grindlay, 2000)
Write:	<<[CCG2000] XA>> <<[CCG2000] Star A>>
N:	3+3
Object:	(X) + * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations reveal 3 distinct X-ray sources within the core of ome Cen, (Nos XA-XC). Stars (Nos A-C) are possible counterpart of each X-ray source.
in source:	ome Cen = NGC 5139
Ref:	=2000ApJ...532..461C
by	CARSON J.E. , COOL A.M., GRINDLAY J.E.
	Astrophys. J., 532, 461-466 (2000)
	Optical identification of faint X-ray sources in the core of ω Centauri.
o	Fig.1: <[CCG2000] XA> (Nos XA-XC). Fig.2, Table 1: <[CCG2000] Star A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCG2002]
[CCG2002]	(Chen+Chu+Gruendl+, 2002)= ([CCG2002a])
Write:	<<[CCG2002] NN>> <<[CCG2002] Shell N>>
N:	28+3
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	HST observations of NGC 5471B in M 101.
in source:	M 101
Ref:	=2002AJ....123.2462C
by	CHEN C.-H.R. , CHU Y.-H., GRUENDL R., LAI S.-P., WANG Q.D.
	Astron. J., 123, 2462-2472 (2002)
	A critical examination of hypernova remnant candidates in M101. II. NGC 5471B.
o	Fig.3, Table 2: <[CCG2002] NN> (Nos 1-28). Table 3: <[CCG2002] Shell N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCG2002a]
[CCG2002a]	(Chen+Chu+Gruendl+, 2002)
*****	Avoid the usage of [CCG2002a], prefer [CCG2002]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCG2002b]
[CCG2002b]	(Cairos+Caon+Grcia-Lorenzo+, 2002) (Not yet in Simbad)
Write:	<<[CCG2002b] Region A>> <<[CCG2002b] Knot NN>>
N:	2+16
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Note:	N=2 starburst regions A and B in Mrk 370. N=16 individual knots.
in source:	Mrk 370
Ref:	=2002ApJ...577..164C
by	CAIROS L.M. , CAON N., GARCIA-LORENZO B., VILCHEZ J.M., MUNOZ-TUNON C.
	Astrophys. J., 577, 164-182 (2002)
	Spectrophotometric observations of blue compact dwarf galaxies: Markarian 370.
o	p. 175 : Haro 3 = [H56] 3 (= NGC 3353)
o	Fig.2: <[CCG2002b] Region A> (Nos A-B). Table 4: <[CCG2002b] Knot NN> (Nos 1-16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCG2007]
[CCG2007]	(Codella+Cabrit+Gueth+, 2007)
Write:	<<[CCG2007] MMN>>
N:	2
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	IRAM PdB Interferometer 1.4mm continuum observations of the field of the HH 212 outflow.
in source:	HH 212
Ref:	=2007A&A...462L..53C
by	CODELLA C. , CABRIT S., GUETH F., CESARONI R., BACCIOTTI F., LEFLOCH B., McCAUGHREAN M.J.
	Astron. Astrophys., 462L, 53-56 (2007)
	A highly-collimated SiO jet in the HH212 protostellar outflow.
o	Fig.1c: <[CCG2007] MMN> (Nos MM1, MM2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCG2009]
[CCG2009]	(Chen+Chu+Gruendl+, 2009)
Write:	<<[CCG2009] JHHMMSS.s+DDMMSS.s>>
N:	17002
Object:	(IR) + Poss. YSO (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC and MIPS observations. NIR and optical imaging at the CTIO Blanco 4m telescope. Use of archival HST images.
in source:	NAME MAGELLANIC CLOUDS:NAME LMC:LHA 120-N 44 = LHA 120-N 44
Ref:	=2009ApJ...695..511C
by	CHEN C.-H.R. , CHU Y.-H., GRUENDL R.A., GORDON K.D., HEITSCH F.
	Astrophys. J., 695, 511-541 (2009)
	Spitzer view of young massive stars in the Large Magellanic Cloud H II complex N 44.
o	Table 2: <[CCG2009] JHHMMSS.s+DDMMSS.s> N=17002.
=E=	Catalogue in electronic form as <J/ApJ/695/511/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCG2012]
[CCG2012]	(Clowes+Campusano+Graham+, 2012)
Write:	<<[CCG2012] Uz.zz>>
N:	3
Object:	Large Quasar Group (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Use of DR7QSO catalogue of the SDSS to determine N=3 large quasar groups. In the format, the letter U refers to a connected unit of quasars, and the number refers to the mean redshift. See also [CHR2013].
Ref:	=2012MNRAS.419..556C
by	CLOWES R.G. , CAMPUSANO L.E., GRAHAM M.J., SOCHTING I.K.
	Mon. Not. R. Astron. Soc., 419, 556-565 (2012)
	Two close large quasar groups of size ~ 350 mpc at z ~ 1.2.
o	<[CCG2012] UZ.zz> (Nos U1.28, U1.11, U1.54).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCG2013]
[CCG2013]	(Contreras Pena+Catelan+Grundhal+, 2013) (Not yet in Simbad)
Write:	<<[CCG2013] ID-NNNN>>
N:	8126
Object:	* (SIMBAD class: Star)
Note:	CTIO 0.9m telescope BVI photometry of N=8126 stars in NGC 6402.
in source:	NGC 6402 = M 14
Ref:	=2013AJ....146...57C
by	CONTRERAS PENA C. , CATELAN M., GRUNDAHL F., STEPHENS A.W., SMITH H.A.
	Astron. J., 146, 57 (2013)
	The globular cluster NGC 6402 (M14). I. A new BV color-magnitude diagram.
o	Table 1: <[CCG2013] ID-NNNN> (Nos 0001-8126).
=E=	Catalogue in electronic form as <J/AJ/146/57/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCG2013]
[CCG2013]	(Contreras Pena+Catelan+Grundhal+, 2013)= ([CCG2013a]) (Not yet in Simbad)
Write:	<<[CCG2013] ID-NNNN>>
N:	8126
Object:	* (SIMBAD class: Star)
Note:	CTIO 0.9m telescope BVI photometry of N=8126 stars in NGC 6402.
in source:	NGC 6402 = M 14
Ref:	=2013AJ....146...57C
by	CONTRERAS PENA C. , CATELAN M., GRUNDAHL F., STEPHENS A.W., SMITH H.A.
	Astron. J., 146, 57 (2013)
	The globular cluster NGC 6402 (M14). I. A new BV color-magnitude diagram.
o	Table 1: <[CCG2013] ID-NNNN> (Nos 0001-8126).
=E=	Catalogue in electronic form as <J/AJ/146/57/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCG2013a]
[CCG2013a]	(Contreras Pena+Catelan+Grundhal+, 2013) (Not yet in Simbad)
*****	Avoid the usage of [CCG2013a], prefer [CCG2013]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCG2013b]
[CCG2013b]	(Cusano+Clementini+Garofalo+, 2013)
Write:	<<[CCG2013b] VNN>>
N:	39
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	Large Binocular Telescope photometry of Andromeda XIX for identification of N=39 pulsating variable stars. See also [CGC2015] and [CGC2016].
in source:	And XIX
Ref:	=2013ApJ...779....7C
by	CUSANO F. , CLEMENTINI G., GAROFALO A., CIGNONI M., FEDERICI L., MARCONI M., MUSELLA I., RIPEPI V., BOUTSIA K., FUMANA M., GALLOZZI S., TESTA V.
	Astrophys. J., 779, 7 (2013)
	Dwarf spheroidal satellites of M31. I. Variable stars and stellar populations in Andromeda XIX.
o	Table 2: <[CCG2013b] VNN> N=39.
=E=	Catalogue in electronic form as J/ApJ/779/7
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCG99]
[CCG99]	(Calzetti+Conselice+Gallagher III+, 1999) (Not yet in Simbad)
Write:	<<[CCG99] NGC 5236 A>>
N:	4
Object:	Region (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Fig.4c: (Nos A-D), 4 regions in NGC 5236. A is an Arc, B a clump, C and D are knots.
in source:	NGC 5236 = M 83
Ref:	=1999AJ....118..797C
by	CALZETTI D. , CONSELICE C.J., GALLAGHER III J.S., KINNEY A.L.
	Astron. J., 118, 797-816 (1999)
	The structure and morphology of the ionized gas in starburst galaxies: NGC 5253/5236.
o	Fig.4c: <[CCG99] NGC 5236 A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CCGCS
CCGCS	(Catalog of Cool Gal. Carbon *)
**	catalog: use CGCS
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CCH2004]
[CCH2004]	(Capak+Cowie+Hu+, 2004)
Write:	<<[CCH2004] R NNNNN>> <<[CCH2004] z' NNNN>>
N:	47450+1408
Note:	Deep multicolor imaging survey of 0.2 square degree centered on the Hubble Deep Field North. Data were collected on the NOAO 4m Mayall telescope, the National Astronomical Observatory of Japan 8.2m Subaru telescope and the University of Hawaii 2.2m telescope.
in source:	NAME HDFN
Ref:	=2004AJ....127..180C
by	CAPAK P. , COWIE L.L., HU E.M., BARGER A.J., DICKINSON M., FERNANDEZ E., GIAVALISCO M., KOMIYAMA Y., KRETCHMER C., McNALLY C., MIYAZAKI S., OKAMURA S., STERN D.
	Astron. J., 127, 180-198 (2004)
	A deep wide-field, optical, and near-infrared catalog of a large area around the Hubble Deep Field North.
o	<[CCH2004] R NNNNN> N=47450 among (Nos 386-66405). <[CCH2004] z' NNNN> N=1408 among (Nos 200-2669).
=E=	Catalogue in electronic form as J/AJ/127/180
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCH78]
[CCH78]	(Cowley+Crampton+Hutchings, 1978)
Write:	<<[CCH78] LMC X-N NN>> <<[CCH78] 4U HHMM+DD NN>> <<[CCH78] 2S HHMM+DDd NN>> <<[CCH78] H HHMM+DD NN>> <<[CCH78] MX HHMM+DD NN>> <<[CCH78] 2A HHMM+DDd NN>>
N:	308
Object:	* (SIMBAD class: Star)
Note:	Stars in the field of 20 X-ray sources Figs 1-5: Maps
Ref:	=1978AJ.....83.1619C
by	COWLEY A.P. , CRAMPTON D., HUTCHINGS J.B.
	Astron. J., 83, 1619-1638 (1978)
	Transmission grating spectroscopy of X-ray source fields.
o	p. 1635, 1636 format A = [PPM75] 3U
o	Table II: <[CCH78] LMC X-N NN>, <[CCH78] 4U HHMM+DD NN>, <[CCH78] 2S HHMM+DDd NN>, <[CCH78] H HHMM+DD NN>, <[CCH78] MX DDMM+DD NN>, <[CCH78] 2A HHMM+DDd NN>, N=308
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCH82]
[CCH82]	(Condon+Condon+Hazard, 1985)
Write:	<<[CCH82] HHMM+DDMMA>>
N:	178
Object:	Radio (SIMBAD class: Radio = Radio Source)
Note:	The format 'HHMM+DDMM' is truncated. The format 'HHMM+DDMMA' is the average coordinates of the two components A and B Paper I, see also papers II: [CM82] and III: [CCH85]
Ref:	=1982AJ.....87..739C
by	CONDON J.J. , CONDON M.A., HAZARD C.
	Astron. J., 87, 739-750 (1982)
	Complete samples of active extragalactic objects. I. A 1411 MHz VLA survey centered on α = 12h04m, δ = +11D30.
o	<[CCH82] HHMM+DDMMA> N=178
=E=	Catalogue in electronic form as J/AJ/87/739
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCH84]
[CCH84]	(Cowley+Crampton+Hutchings+, 1984) (Not yet in Simbad)
Write:	<<[CCH84] CAL NN Star N>> <<[CCH84] CAL A Star N>>
N:	17+31
Object:	* (SIMBAD class: Star)
Note:	Stars in the field of CAL X-ray sources, possible counterpart of the X-ray.
Ref:	=1984ApJ...286..196C
by	COWLEY A.P. , CRAMPTON D., HUTCHINGS J.B., HELFAND D.J., HAMILTON T.T., THORSTENSEN J.R., CHARLES P.A.
	Astrophys. J., 286, 196-208 (1984)
	Optical counterparts of the Large Magellanic Cloud X-ray point sources.
o	Table 1: <CAL A> (Nos A-G), Nos C and D missing. Fig.2: <[CCH84] CAL NN Star N>, <[CCH84] CAL A Star N>, N=17.
Ref:	=1985AJ.....90...43C
by	CRAMPTON D. , COWLEY A.P., THOMPSON I.B., HUTCHINGS J.B.
	Astron. J., 90, 43-48 (1985)
	Further spectroscopy of LMC X-ray candidates.
o	Table I, Fig.3: <[<[CCH84] CAL NN Star N>, <[CCH84] CAL A Star N>, N=31.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCH85]
[CCH85]	(Coleman+Condon+Hazard, 1985)
Write:	<<[CCH85] HHMM+DDMMA>>
N:	208
Object:	Radio (SIMBAD class: Radio = Radio Source)
Note:	The format 'HHMM+DDMM' is truncated. The format 'HHMM+DDMMA' is the average coordinates of the two components A and B Paper III, see also papers I: [CCH82] and II: [CM82]. 96 S
Ref:	=1985AJ.....90.1437C
by	COLEMAN P.H. , CONDON J.J., HAZARD C.
	Astron. J., 90, 1437-1448 (1985)
	Complete samples of active extragalactic objects. III. A 1411 MHz VLA survey.
o	<[CCH85] HHMM+DDMMA> N=208
=E=	Catalogue in electronic form as J/AJ/90/1437
Details on Acronym: [CCH87]
[CCH87]	(Crampton+Cowley+Hartwick, 1987)
Write:	<<[CCH87] HHMM.m+DDMMA>> <<[CCH87] HHMM.m+DDd>>
N:	159
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Note:	See also [CR82], [CP83], [CSC85], [CC87], [CCS88], [CCH90], [CCH91], [CCH92], [CGC97]
Ref:	=1987ApJ...314..129C
by	CRAMPTON D. , COWLEY A.P., HARTWICK F.D.A.
	Astrophys. J., 314, 129-144 (1987)
	The space distribution of faint quasars from the CFHT survey.
o	Table 1A: <[CCH87] HHMM.m+DDMMA>, <[CCH87] HHMM.m+DDd> N=159
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCH90]
[CCH90]	(Crampton+Cowley+Hartwick, 1990)
Write:	<<[CCH90] HHMM.m+DDMM>>
N:	106
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Note:	See also [CR82], [CP83], [CSC85], [CC87], [CCH87], [CCS88], [CCH91], [CCH92], [CGC97]
Ref:	=1990AJ....100...47C
by	CRAMPTON D. , COWLEY A.P., HARTWICK F.D.A.
	Astron. J., 100, 47-55 (1990)
	Redshifts of quasars in the CFHT/MMT survey. III.
o	Table 1A: <[CCH90] HHMM.m+DDMM> N=106
=E=	Catalogue in electronic form as VII/143
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCH91]
[CCH91]	(Crampton+Cowley+Hartwick+, 1991)
Write:	<<[CCH91] HHMM.m+DDMM>>
N:	145
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Note:	See also [CR82], [CP83], [CSC85], [CC87], [CCH87], [CCS88], [CCH90], [CCH92], [CGC97]
Ref:	=1991AJ....101.1183C
by	CRAMPTON D. , COWLEY A.P., HARTWICK F.D.A., CARTLEDGE S.
	Astron. J., 101, 1183-1186 (1991)
	Quasar candidates near 1057+01.
o	Table 2: <[CCH91] HHMM.m+DDMM> N=145
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCH92]
[CCH92]	(Crampton+Cowley+Hartwick+, 1992)
Write:	<<[CCH92] HHMM.m+DDMM>>
N:	488+14+8
Object:	Poss. QSO + Em. G + WD (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	See also [CR82], [CP83], [CSC85], [CC87], [CCH87], [CCS88], [CCH90], [CCH91], [CGC97]
Ref:	=1992AJ....104.1706C
by	CRAMPTON D. , COWLEY A.P., HARTWICK F.D.A., KO P.W.
	Astron. J., 104, 1706-1713 (1992)
	Canada-France-Hawaii telescope blue grens quasar candidates.
o	Tables 2, 3: <[CCH92] HHMM.m+DDMM> N=510
=E=	Catalogue in electronic form as J/AJ/104/1706
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCH96]
[CCH96]	(Cohen+Cowie+Hogg+, 1996)
Write:	<<[CCH96] JHHMMSS.s+DDMMSS.s>> <<[CCH96] JHHMMSS.ss+DDMMSS.s>>
N:	152
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Hubble Deep Field redshift sample. See also [HCB98].
in source:	NAME HDFN
Ref:	=1996ApJ...471L...5C
by	COHEN J.G. , COWIE L.L., HOGG D.W., SONGAILA A., BLANDFORD R., HU E.M., SHOPBELL P.
	Astrophys. J., 471, 5-10 (1996)
	Redshift clustering in the Hubble Deep Field.
o	Table 1: <[CCH96] JHHMMSS.s+DDMMSS.s>, <[CCH96] JHHMMSS.ss+DDMMSS.s>, N=152
=E=	Catalogue in electronic form as J/ApJ/471/L5
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCI2009]
[CCI2009]	(Collins+Chapman+Irwin+, 2009)
Write:	<<[CCI2009] JHHMMSS.s+DDMMSS.s>>
N:	8
Object:	RGB* (SIMBAD class: RGB* = Red Giant Branch star)
Stat:	is completely incorporated in Simbad
Note:	Keck II DEIMOS observations of RGB stars in M31WFS C4.
in source:	M31WFS C4
Ref:	=2009MNRAS.396.1619C
by	COLLINS M.L.M. , CHAPMAN S.C., IRWIN M., IBATA R., MARTIN N.F., FERGUSON A.M.N., HUXOR A., LEWIS G.F., MacKEY A.D., McCONNACHIE A.W., TANVIR N.
	Mon. Not. R. Astron. Soc., 396, 1619-1628 (2009)
	A spectroscopic survey of EC4, an extended cluster in Andromeda's halo.
o	Table 1: <[CCI2009] JHHMMSS.s+DDMMSS.s> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCI2010]
[CCI2010]	(Collins+Chapman+Irwin+, 2010)
Write:	<<[CCI2010] JHHMMSS.ss+DDMMSS.s>>
N:	5+8+3+9
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Subaru Suprime-Cam photometry and Keck II DEIMOS spectroscopy of N=5+8+3+9 stars in the faint M31 satellite galaxies And IX, And XI, And XII, and And XIII.
in source:	And IX
in source:	And XI
in source:	And XII
in source:	And XIII
Ref:	=2010MNRAS.407.2411C
by	COLLINS M.L.M. , CHAPMAN S.C., IRWIN M.J., MARTIN N.F., IBATA R.A., ZUCKER D.B., BLAIN A., FERGUSON A.M.N., LEWIS G.F., McCONNACHIE A.W., PENARRUBIA J.
	Mon. Not. R. Astron. Soc., 407, 2411-2433 (2010)
	A Keck/DEIMOS spectroscopic survey of the faint M31 satellites AndIX, AndXI, AndXII and AndXIII.
o	Tables 2-5: <[CCI2010] JHHMMSS.ss+DDMMSS.s> N=5+8+3+9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCJ2005]
[CCJ2005]	(Chen+Chu+Johnson, 2005)
Write:	<<[CCJ2005] NGC NNNN NN>>
N:	12+25+19
Object:	Poss. Stellar Cluster (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of 3 giant HII regions in M101. Search for candidate clusters.
in source:	NGC 5461
in source:	NGC 5462
in source:	NGC 5471
Ref:	=2005ApJ...619..779C
by	CHEN C.-H.R. , CHU Y.-H., JOHNSON K.E.
	Astrophys. J., 619, 779-799 (2005)
	Clusters in the luminous giant H II regions in M 101.
o	Table 3: <[CCJ2005] NGC 5461 NN> (Nos 1-12). Table 4: <[CCJ2005] NGC 5462 NN> (Nos 1-25). Table 5: <[CCJ2005] NGC 5471 NN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCJ2015]
[CCJ2015]	(Cao+Covone+Jullo+, 2015)= ([CCJ2015a])
Write:	<<[CCJ2015] GalN>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Note:	N=3 galaxies, members of the galaxy cluster ACO 2667. Use of HST ACS and VLT ISAAC imaging data.
in source:	ACO 2667
Ref:	=2015AJ....149....3C
by	CAO S. , COVONE G., JULLO E., RICHARD J., IZZO L., ZHU Z.-H.
	Astron. J., 149, 3 (2015)
	Source-plane reconstruction of the giant gravitational arc in A2667: a candidate Wolf-Rayet galaxy at z ~ 1.
o	Fig. 1, Table 1: <[CCJ2015] GalN> (Nos Gal2-Gal4).
o	in Table 1, the directions for RA are reversed.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCJ2015a]
[CCJ2015a]	(Cao+Covone+Jullo+, 2015)
*****	Avoid the usage of [CCJ2015a], prefer [CCJ2015]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCJ2015b]
[CCJ2015b]	(Capak+Carilli+Jones+, 2015)
Write:	<<[CCJ2015b] HZNN>> <<[CCJ2015b] HZ5a>> <<[CCJ2015b] HZ8W>>
N:	10+1+1
Object:	G (SIMBAD class: Galaxy)
Note:	ALMA band 7 continuum observations of N=12 galaxies in the COSMOS field.
in source:	NAME COSMOS Field
Ref:	=2015Natur.522..455C
by	CAPAK P.L. , CARILLI C., JONES G., CASEY C.M., RIECHERS D., SHETH K., CAROLLO C.M., ILBERT O., KARIM A., LEFEVRE O., LILLY S., SCOVILLE N., SMOLCIC V., YAN L.
	Natur, 522, 455-458 (2015)
	Galaxies at redshifts 5 to 6 with systematically low dust content and high [C II] emission.
o	<[CCJ2015b] HZNN> (Nos 1-10), <[CCJ2015b] HZ5a> N=1, <[CCJ2015b] HZ8W> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCK2016]
[CCK2016]	(Cromartie+Camilo+Kerr+, 2016)
Write:	<<[CCK2016] P7R4 JHHMM+DDMM>>
N:	2
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	N=2 unidentified gamma-ray sources from the Fermi LAT four year point source catalog, candidates to a search for radio millisecond pulsars with the Arecibo telescope.
Ref:	=2016ApJ...819...34C
by	CROMARTIE H.T. , CAMILO F., KERR M., DENEVA J.S., RANSOM S.M., RAY P.S., FERRARA E.C., MICHELSON P.F., WOOD K.S.
	Astrophys. J., 819, 34 (2016)
	Six new millisecond pulsars from Arecibo searches of Fermi γ-ray sources.
o	Tables 1+4: <[CCK2016] P7R4 JHHMM+DDMM> (No. J1250+3118, J1909+2102).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCK2018]
[CCK2018]	(Cotton+Condon+Kellermann+, 2018)
Write:	<<[CCK2018] JHHMMSS.sss+DDMMSS.ss>>
N:	792
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Karl G. Jansky VLA 3GHz observations of N=792 radio sources in the Lockman Hole North.
in source:	NAME Lockman Hole
Ref:	=2018ApJ...856...67C
by	COTTON W.D. , CONDON J.J., KELLERMANN K.I., LACY M., PERLEY R.A., MATTHEWS A.M., VERNSTROM T., SCOTT D., WALL J.V.
	Astrophys. J., 856, 67-67 (2018)
	The angular size distribution of µJy radio sources.
o	Table 2: <[CCK2018] JHHMMSS.sss+DDMMSS.ss> N=792.
=E=	Catalogue in electronic form as J/ApJ/856/67
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCL2001]
[CCL2001]	(Castets+Ceccarelli+Loinard+, 2001)= (CCLCL)
Write:	<<[CCL2001] HEN>>
N:	2
Object:	Feature (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=2 H2CO structures in the field of IRAS 16293-2422. See also [HMU2001].
in source:	IRAS 16293-2422
Ref:	=2001A&A...375...40C
by	CASTETS A. , CECCARELLI C., LOINARD L., CAUX E., LEFLOCH B.
	Astron. Astrophys., 375, 40-53 (2001)
	Multiple shocks around the low-luminosity protostar IRAS 16293-2422.
o	In ref list 1996A&A.315L.181L instead of 1996A&A.315.181L.
o	Fig.2: <[CCL2001] HEN> (Nos HE1, HE2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCL2007]
[CCL2007]	(Carrasco+Cypriano+Lima Neto+, 2007)
Write:	<<[CCL2007] NNNN>>
N:	77
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Gemini South GMOS observations of the galaxy cluster RX J1117.4+0743.
in source:	RX J1117.4+0743 = [VMF98] 97
Ref:	=2007ApJ...664..777C
by	CARRASCO E.R. , CYPRIANO E.S., LIMA NETO G.B., CUEVAS H., SODRE L.Jr, MENDES DE OLIVEIRA C., RAMIREZ A.
	Astrophys. J., 664, 777-790 (2007)
	Witnessing the formation of a galaxy cluster at z = 0.485: optical and X-ray properties of RX J1117.4+0743 ([VMF 98] 097).
o	Tablez 1: <[CCL2007] NNNN> N=77 among (Nos 1-3054).
=E=	Catalogue in electronic form as J/ApJ/664/777
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCL2008]
[CCL2008]	(Capak+Carilli+Lee+, 2008)
Write:	<<[CCL2008] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	smm G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck II DEIMOS spectroscopy of a submillimeter galaxy at z=4.547.
Ref:	=2008ApJ...681L..53C
by	CAPAK P. , CARILLI C.L., LEE N., ALDCROFT T., AUSSEL H., SCHINNERER E., WILSON G.W., YUN M.S., BLAIN A., GIAVALISCO M., ILBERT O., KARTALTEPE J., LEE K.-S., McCRACKEN H., MOBASHER B., SALVATO M., SASAKI S., SCOTT K.S., SHETH K., SHIOYA Y., THOMPSON D., ELVIS M., SANDERS D.B., SCOVILLE N.Z., TANAGUCHI Y.
	Astrophys. J., 681L, 53-56 (2008)
	Spectroscopic confirmation of an extreme starburst at redshift 4.547.
o	<[CCL2008] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCL2013]
[CCL2013]	(Carollo+Cibinel+Lilly+, 2013)
Write:	<<[CCL2013] 2PIGG wNNNN NNNA>>
N:	1656
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=1656 galaxies members of 141 2PIGG groups, as part of the Zurich Environmental Study (ZENS). The ZENS sample is extracted from the two-degree Field Galaxy Redshift Survey (2dFGRS).
Ref:	=2013ApJ...776...71C
by	CAROLLO C.M. , CIBINEL A., LILLY S.J., MINIATI F., NORBERG P., SILVERMAN J.D., VAN GORKOM J., CAMERON E., FINOGUENOV A., PENG Y., PIPINO A., RUDICK C.S.
	Astrophys. J., 776, 71 (2013)
	The Zurich Environmental Study of galaxies in groups along the cosmic web. I. Which environment affects galaxy evolution?
o	Table 4: <[CCL2013] 2PIGG wNNNN NNNA> N=1656.
=E=	Catalogue in electronic form as J/ApJ/776/71
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCL2014]
[CCL2014]	(Cerulo+Couch+Lidman+, 2014)
Write:	<<[CCL2014] XMM1229 NNN>> <<[CCL2014] FORS2 NNNN>>
N:	53+6
Object:	G (SIMBAD class: Galaxy)
Note:	HST ACS and WFC3, VLT FORS2 and HAWK-I, NTT SofI observations of N=53+6 red sequence galaxies in the distant cluster XMMU J229.4+0151
in source:	2XMM J122929.1+015131
Ref:	=2014MNRAS.439.2790C
by	CERULO P. , COUCH W.J., LIDMAN C., DELAYE L., DEMARCO R., HUERTAS-COMPANY M., MEI S., SANCHEZ-JANSSEN R.
	Mon. Not. R. Astron. Soc., 439, 2790-2812 (2014)
	The morphological transformation of red sequence galaxies in the distant cluster XMMU J1229+0151.
o	Figs A1-A4: Table 3: <[CCL2014] XMM1229 NNN> N=53 among (Nos 73-502), <[CCL2014] FORS2 NNNN> N=6 among (Nos 4661-5001).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CCLCL
CCLCL	(Castets+Ceccarelli+Loinard+Caux+Lefloch)
*****	Avoid the usage of CCLCL, prefer [CCL2001]
Origin	of the Acronym: L (2004A&A...413..609W)
Details on Acronym: CCM
CCM	(Carranza+Crillon+Monnet)
Write:	<<CCM A>> <<CCM NNNA>>
N:	1+160
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	One HII region format 'A', 109 HII region (Nos 1-109) + 51 HII region format NNNA
in source:	M 51 = NGC 5194
Ref:	=1969A&A.....1..479C
by	CARRANZA G. , CRILLON R., MONNET G.
	Astron. Astrophys., 1, 479-491 (1969)
	Etude cinematique de l'hydrogene ionise dans M 51.
o	<CCM A> N=1, <CCM NNNA> (Nos 1-109), N=160
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CCM2006]
[CCM2006]	(Coppin+Chapin+Mortier+, 2006)= (LH) = (Lock850) = (SHADES) = (SXDF850)
Write:	<<[CCM2006] Lock850.NNN>> <<[CCM2006] SXDF850.NNN>>
N:	60+60
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	SCUBA Half-Degree Extragalactic survey (SHADES).
in source:	NAME Lockman Hole
in source:	NAME SXDF
Ref:	=2006MNRAS.372.1621C
by	COPPIN K. , CHAPIN E.L., MORTIER A.M.J., SCOTT S.E., BORYS C., DUNLOP J.S., HALPERN M., HUGHES D.H., POPE A., SCOTT D., SERJEANT S., WAGG J., ALEXANDER D.M., ALMAINI O., ARETXAGA I., BABBEDGE T., BEST P.N., BLAIN A., CHAPMAN S., CLEMENTS D.L., CRAWFORD M., DUNNE L., EALES S.A., EDGE A.C., FARRAH D., GAZTANAGA E., GEAR W.K., GRANATO G.L., GREVE T.R., FOX M., IVISON R.J., JARVIS M.J., JENNESS T., LACEY C., LEPAGE K., MANN R.G., MARSDEN G., MARTINEZ-SANSIGRE A., OLIVER S., PAGE M.J., PEACOCK J.A., PEARSON C.P., PERCIVAL W.J., PRIDDEY R.S., RAWLINGS S., ROWAN-ROBINSON M., SAVAGE R.S., SEIGAR M., SEKIGUCHI K., SILVA L., SIMPSON C., SMAIL I., STEVENS J.A., TAKAGI T., VACCARI M., VAN KAMPEN E., WILLOTT C.J.
	Mon. Not. R. Astron. Soc., 372, 1621-1652 (2006)
	The SCUBA Hα-Degree Extragalactic Survey - II. Submillimetre maps, catalogue and number counts.
o	Table 2, col(1): <SHADES JHHMMSS+DDMMSS> N=120, = Table 2, col(2): <[CCM2006] Lock850.NNN> N=60 among (Nos 1-100) or <[CCM2006] SXDF850.NNN> N=60 among (Nos 1-119).
=E=	Catalogue in electronic form as J/MNRAS/372/1621
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCM2020]
[CCM2020]	(Ciurlo+Campbell+Morris+, 2020)
Write:	<<[CCM2020] GN>>
N:	4
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Keck OSIRIS and NIRC2 observations of N=4 "G sources", orbiting Sgr A*. See also [BSA2012] for G1 and G2.
in source:	NAME Galactic Center
Ref:	=2020Natur.577..337C
by	CIURLO A. , CAMPBELL R.D., MORRIS M.R., DO T., GHEZ A.M., HEES A., SITARSKI B.N., KOSMO O'NEIL K., CHU D.S., MARTINEZ G.D., NAOZ S., STEPHAN A.P.
	Natur, 577, 337-340 (2020)
	A population of dust-enshrouded objects orbiting the Galactic black hole.
o	<[CCM2020] GN> (Nos G3-G6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCM2021]
[CCM2021]	(Corbelli+Mannucci+Thilker+, 2021)
Write:	<<[CCM2021] C1a>> <<[CCM2021] C2Ea>>
N:	4+4
Object:	HII + Poss. PN (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	VLT MUSE observations of N=4 HII regions and N=1 planetary nebula candidate in the field of the HI clumps [SST86] 1 and [SST86] 2E, in the Leo ring. Use of GALEX and HST archival data.
in source:	NAME Leo Ring
in source:	[SST86] 1
in source:	[SST86] 2E
Ref:	=2021ApJ...908L..39C
by	CORBELLI E. , CRESCI G., MANNUCCI F., THILKER D., VENTURI G.
	Astrophys. J., 908L, 39-39 (2021)
	Heavy elements unveil the non-primordial origin of the giant H I Ring in Leo.
o	Fig. 1, Tables 1-2: <[CCM2021] CNWa> (Nos C1a-C1c, C2Ea-C2Eb).
Ref:	=2021A&A...651A..77C
by	CORBELLI E. , MANNUCCI F., THILKER D., CRESCI G., VENTURI G.
	Astron. Astrophys., 651A, 77-77 (2021)
	Gaseous nebulae and massive stars in the giant H I ring in Leo.
o	Fig. 8, Table 2: <[CCM2021] CNWa> (Nos C2Ec-C2Ef) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCO2011]
[CCO2011]	(Cameron+Carollo+Oesch+, 2011)
Write:	<<[CCO2011] UDFNNNN>> <<[CCO2011] ERSNNNN>>
N:	1052+3078
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Catalogs of N=1052+3078 sources. Use of HST WFC3 observations of the Hubble Ultra Deep Field 2009 (HUDF2009) and Early Release Science (GOODS-South) fields.
Ref:	=2011ApJ...743..146C
by	CAMERON E. , CAROLLO C.M., OESCH P.A., BOUWENS R.J., ILLINGWORTH G.D., TRENTI M., LABBE I., MAGEE D.
	Astrophys. J., 743, 146 (2011)
	Active and passive galaxies at z ~ 2: rest-frame optical morphologies with WFC3.
o	<[CCO2011] UDFNNNN> (Nos 1-1052). <[CCO2011] ERSNNNN> (Nos 1-3078).
=E=	Catalogue in electronic form as <J/ApJ/743/146/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CCOS
CCOS	(Centaurus Compact Object Source)
Write:	<<CCOS JHHMM.mm+DDMM.mm>>
N:	27
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	VLT VIMOS observations of the Centaurus cluster: N=27 compact objects with radial velocities consistent with them being cluster members.
in source:	ACO 3526 = Centaurus Cluster
Ref:	=2007A&A...472..111M
by	MIESKE S. , HILKER M., JORDAN A., INFANTE L., KISSLER-PATIG M.
	Astron. Astrophys., 472, 111-119 (2007)
	A search for ultra-compact dwarf galaxies in the Centaurus galaxy cluster.
o	Table 1: <CCOS JHHMM.mm+DDMM.mm> N=27.
=E=	Catalogue in electronic form as J/A+A/472/111
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CCP2009]
[CCP2009]	(Cairos+Caon+Papaderos+, 2009) (Not yet in Simbad)
Write:	<<[CCP2009] N>>
N:	6
Object:	Star Forming Region (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Calar Alto 3.5m telescope PMAS observations of N=6 star-forming regions in the blue compact dwarf MrK 409.
in source:	Mrk 409 = NGC 3011
Ref:	=2009ApJ...707.1676C
by	CAIROS L.M. , CAON N., PAPADEROS P., KEHRIG C., WEILBACHER P., ROTH M.M., ZURITA C.
	Astrophys. J., 707, 1676-1690 (2009)
	New light in star-forming dwarf galaxies: the PMAS integral field view of the blue compact dwarf galaxy Mrk 409.
o	Fig. 1, Tables 2-4: <[CCP2009] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCP2013]
[CCP2013]	(Cao+Covone+Paolillo+, 2013) (Not yet in Simbad)
Write:	<<[CCP2013] A>>
N:	4
Object:	Grav. lensed image of a G (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy)
Note:	N=4 gravitationally lensed images of background galaxy. Use of HST ACS, Subaru SuprimeCam, XMM, Chandra data, and spectroscopic data from zCOSMOS.
Ref:	=2013RAA....13...15C
by	CAO S. , COVONE G., PAOLILLO M., ZHU Z.-H.
	RAA, 13, 15-27 (2013)
	A multi-wavelength study of the gravitational lens COSMOS J095930+023427.
o	Fig. 1, Table 1: <[CCP2013] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCP99]
[CCP99]	(Cesarsky+Cox+Pineau des Forets+, 1999) (Not yet in Simbad)
Write:	<<[CCP99] Peak A>>
N:	3
Object:	H2 emission (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	T.1: N=3 H2 emission peaks in IC 443.
in source:	IC 443
Ref:	=1999A&A...348..945C
by	CESARSKY D. , COX P., PINEAU DES FORETS G., VAN DISHOECK E.F., BOULANGER F., WRIGHT C.M.
	Astron. Astrophys., 348, 945-949 (1999)
	ISOCAM spectro-imaging of the H_{2} rotational lines in the supernova remnant IC 443.
o	p.945: Clump G = [HDS86] IC 443G.
o	Table 1, Fig.3: <[CCP99] Peak A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CCPC
CCPC	(Candidate Cluster and Protocluster Catalog (CCPC))
Write:	<<CCPC -zzz-NNN>>
N:	12+31+173
Object:	Poss. Cluster of G (SIMBAD class: ClG_Candidate = Cluster of Galaxies Candidate)
Note:	Identification of N=12+31 galaxy protoclusters at z>2.74.
Ref:	=2016ApJ...817..158F
by	FRANCK J.R. , McGAUGH S.S.
	Astrophys. J., 817, 158 (2016)
	The candidate cluster and protocluster catalog (CCPC) of spectroscopically identified structures spanning 2.74 < z < 3.71.
o	Tables 1-2: <CCPC-zZz-NNN> N=12+31 among (Nos CCPC-z27-001 and CCPC-z37-001).
Ref:	=2016ApJ...833...15F
by	FRANCK J.R. , McGAUGH S.S.
	Astrophys. J., 833, 15-15 (2016)
	The Candidate Cluster and Protocluster Catalog (CCPC) II. Spectroscopically identified structures spanning 2< z < 6.6.
o	Tables 3-5: <CCPC-zZz-NNN> N=173 among (Nos -z20-001 to -z65-005).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CCR2009]
[CCR2009]	(Chilingarian+Cayatte+Revaz+, 2009)
Write:	<<[CCR2009] JHHMMSS.ss+DDMMSS.s>>
N:	21
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=21 compact elliptical galaxies gathered with the Virtual Observatory.
Ref:	=2009Sci...326.1379C
by	CHILINGARIAN I. , CAYATTE V., REVAZ Y., DODONOV S., DURAND D., DURRET F., MICOL A., SLEZAK E.
	Sci, 326, 1379-1382 (2009)
	A population of compact elliptical galaxies detected with the Virtual Observatory.
o	Table S1: <[CCR2009] JHHMMSS.ss+DDMMSS.s> N=21.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCR2011]
[CCR2011]	(Collins+Chapman+Rich+, 2011)
Write:	<<[CCR2011] JHHMMSS.ss+DDMMSS.s>> <<[CCR2011] JHHMMSS.ss+DDMMSS.ss>>
N:	18+34
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Keck I LRIS and Keck II DEIMOS and Subaru Suprime-Cam observations of And V and And VI.
in source:	And V
in source:	And VI
Ref:	=2011MNRAS.417.1170C
by	COLLINS M.L.M. , CHAPMAN S.C., RICH R.M., IRWIN M.J., PENARRUBIA J., IBATA R.A., ARIMOTO N., BROOKS A.M., FERGUSON A.M.N., LEWIS G.F., McCONNACHIE A.W., VENN K.
	Mon. Not. R. Astron. Soc., 417, 1170-1182 (2011)
	The scatter about the `Universal' dwarf spheroidal mass profile: a kinematic study of the M31 satellites And V and And VI.
o	Table 3: <[CCR2011] JHHMMSS.ss+DDMMSS.s> N=18. Table 4: <[CCR2011] JHHMMSS.ss+DDMMSS.ss> N=34.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCR2013]
[CCR2013]	(Collins+Chapman+Rich+, 2013)
Write:	<<[CCR2013] JHHMMSS.ss+DDMMSS.s>>
N:	287 (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Keck I LRIS and Keck II DEIMOS and Subaru Suprime-Cam observations of 295 red giant branch stars in 18 Andromeda dwarf spheroidal (dSph) galaxies.
Ref:	=2013ApJ...768..172C
by	COLLINS M.L.M. , CHAPMAN S.C., RICH R.M., IBATA R.A., MARTIN N.F., IRWIN M.J., BATE N.F., LEWIS G.F., PENARRUBIA J., ARIMOTO N., CASEY C.M., FERGUSON A.M.N., KOCH A., McCONNACHIE A.W., TANVIR N.
	Astrophys. J., 768, 172 (2013)
	A kinematic study of the Andromeda dwarf spheroidal system.
o	Table 3: <[CCR2013] JHHMMSS.ss+DDMMSS.s> N=295.
=E=	Catalogue in electronic form as <J/ApJ/768/172/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCR2014]
[CCR2014]	(Cloutier+Currie+Rieke+, 2014)
Write:	<<[CCR2014] NNNNN>>
N:	13956
Object:	* in stellar cluster (SIMBAD class: Star)
Note:	Spitzer IRAC 3.6µm and 8µm and MIPS 24µm photometric observations of the Double Cluster h and χ Persei. Use of archival 2MASS data. See also [CBK2007b], [CKB2007], [CKR2007], [CKB2008] and [CHI2010].
in source:	h Per Cluster = NGC 869
in source:	chi Per Cluster = NGC 884
Ref:	=2014ApJ...796..127C
by	CLOUTIER R. , CURRIE T., RIEKE G.H., KENYON S.J., BALOG Z., JAYAWARDHANA R.
	Astrophys. J., 796, 127 (2014)
	A deep Spitzer survey of circumstellar disks in the young double cluster, h and χ Persei.
o	Table 1: <[CCR2014] NNNNN> (Nos 1-13956).
=E=	Catalogue in electronic form as J/ApJ/796/127
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CCS
CCS	(Cool Carbon *)
====>	Equivalent to: C*
Details on Acronym: [CCS2010]
[CCS2010]	(Contreras+Catelan+Smith+, 2010)
Write:	<<[CCS2010] VNN>> <<[CCS2010] NVNNN>>
N:	66+179
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	LCO 1.3m Warsaw telescope and CTIO 1.3m telescope observations of the galactic globular cluster M62. In the format, NV stands for New Variable.
in source:	NGC 6266 = M 62
Ref:	=2010AJ....140.1766C
by	CONTRERAS R. , CATELAN M., SMITH H.A., PRITZL B.J., BORISSOVA J., KUEHN C.A.
	Astron. J., 140, 1766-1786 (2010)
	Time-series photometry of globular clusters: M62 (NGC 6266), the most RR Lyrae-rich globular cluster in the Galaxy?
o	Finding charts.
o	Fig. 1, Tables 1-6: <[CCS2010] VNN> N=66 among (Nos V1-V83), <[CCS2010] NVNNN> N=179 among (Nos NV84-NV262).
=E=	Catalogue in electronic form as <J/AJ/140/1766/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCS2021]
[CCS2021]	(Cid Fernandes+Carvalho+Sanchez+, 2021)
Write:	<<[CCS2021] NN>>
N:	59
Object:	Poss. SNR (SIMBAD class: SNRemnant_Candidate = SuperNova Remnant Candidate)
Stat:	is completely incorporated in Simbad
Note:	VLT MUSE observations of N=59 SNR candidates in NGC 4030.
in source:	NGC 4030
Ref:	=2021MNRAS.502.1386C
by	CID FERNANDES R. , CARVALHO M.S., SANCHEZ S.F., DE AMORIM A., RUSCHEL-DUTRA D.
	Mon. Not. R. Astron. Soc., 502, 1386-1400 (2021)
	Detection of supernova remnants in NGC 4030.
o	SN 2015gb is a misprint SN 2015bh.
o	Table 1: <[CCS2021] NN> (Nos 1-59).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCS85]
[CCS85]	(Crampton+Cowley+Schade+, 1985)= (D) = (DAO)
Write:	<<[CCS85] NNN>>
N:	109
Object:	Poss. GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
in source:	M 31 = NGC 224
Ref:	=1985ApJ...288..494C
by	CRAMPTON D. , COWLEY A.P., SCHADE D., CHAYER P.
	Astrophys. J., 288, 494-513 (1985)
	The M 31 globular cluster system.
o	(Erratum) + erratum vol 322, 1074
o	Table 3 is not in Simbad
o	Table 2: <[CCS85] NNN> (Nos 1-109).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCS88]
[CCS88]	(Crampton+Cowley+Schmidtke+, 1988)
Write:	<<[CCS88] HHMM.m+DDMMA>>
N:	777
Object:	Poss. QSO + WD + HII (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Note:	The 1950 right ascension are rounded, not truncated See also [CR82], [CP83], [CSC85], [CC87], [CCH87], [CCH90], [CCH91], [CCH92], [CGC97]
Ref:	=1988AJ.....96..816C
by	CRAMPTON D. , COWLEY A.P., SCHMIDTKE P.C., JANSON T., DURRELL P.
	Astron. J., 96, 816-835 (1988)
	Quasar candidates in two extended CFHT fields : 1338+27 and 1639+40.
o	Table IV: <[CCS88] HHMM.M+DDMMA> N=777
=E=	Catalogue in electronic form as VII/143
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCS92]
[CCS92]	(Clegg+Cordes+Simonetti+, 1992)
Write:	<<[CCS92] HHMM+DDA>> <<[CCS92] HHMM+DDdA>>
N:	76
Object:	Exgl (Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Ref:	=1992ApJ...386..143C
by	CLEGG A.W. , CORDES J.M., SIMONETTI J.H., KULKARNI S.R.
	Astrophys. J., 386, 143-157 (1992)
	Rotation measures of low-latitude extragalactic sources and the magnetoionic structure of the galaxy.
o	<[CCS92] HHMM+DDA> or <[CCS92] HHMM+DDdA> N=76
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCT2010]
[CCT2010]	(Carrasco+Conselice+Trujillo+, 2010)
Write:	<<[CCT2010] NNNNNNNN>>
N:	6
Object:	G (SIMBAD class: Galaxy)
Note:	Gemini-North NIRI/ALTAIR observations of massive galaxies selected from the Palomar Observatory Wide-Field Infrared survey.
Ref:	=2010MNRAS.405.2253C
by	CARRASCO E.R. , CONSELICE C.J., TRUJILLO I.
	Mon. Not. R. Astron. Soc., 405, 2253-2259 (2010)
	Gemini K-band NIRI adaptive optics observations of massive galaxies at 1 < z < 2.
o	Fig. 1, Table 1: <[CCT2010] NNNNNNNN> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCV2000]
[CCV2000]	(Charmandaris+Combes+van der Hulst, 2000)
Write:	<<[CCV2000] SN>>
N:	4
Object:	Region (SIMBAD class: Region = Region defined in the Sky)
Stat:	is completely incorporated in Simbad
Note:	CO observations in shells. N=4 regions in Centaurus A. CO is detected in S1 and S2 corresponding to several HI and stellar shells (see [MQG83]). S3 is a series of pointing along an optical shell. S4 is a single pointing. Map in Fig.1.
in source:	Cen A = NGC 5128
Ref:	=2000A&A...356L...1C
by	CHARMANDARIS V. , COMBES F., VAN DER HULST J.M.
	Astron. Astrophys., 356, 1-4 (2000)
	First detection of molecular gas in the shells of Cen A.
o	Fig.1: <[CCV2000] SN> (Nos S1-S4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCV2011]
[CCV2011]	(Conley+Cooray+Vieira+, 2011)
Write:	<<[CCV2011] HLSW-01>> <<[CCV2011] HLSW-01 N>>
N:	1+4
Object:	Submm G + Grav. lensed image of a G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Herschel SPIRE Science Demonstration Phase and SMA 880mu.m observations of a multiply lensed submillimeter galaxy in the Lockman/SWIRE field.
Ref:	=2011ApJ...732L..35C
by	CONLEY A. , COORAY A., VIEIRA J.D., GONZALEZ SOLARES E.A., KIM S., AGUIRRE J.E., AMBLARD A., AULD R., BAKER A.J., BEELEN A., BLAIN A., BLUNDELL R., BOCK J., BRADFORD C.M., BRIDGE C., BRISBIN D., BURGARELLA D., CARPENTER J.M., CHANIAL P., CHAPIN E., CHRISTOPHER N., CLEMENTS D.L., COX P., DJORGOVSKI S.G., DOWELL C.D., EALES S., EARLE L., ELLSWORTH-BOWERS T.P., FARRAH D., FRANCESCHINI A., FRAYER D., FU H., GAVAZZI R., GLENN J., GRIFFIN M., GURWELL M.A., HALPERN M., IBAR E., IVISON R.J., JARVIS M., KAMENETZKY J., KRIPS M., LEVENSON L., LUPU R., MAHABAL A., MALONEY P.D., MARASTON C., MARCHETTI L., MARSDEN G., MATSUHARA H., MORTIER A.M.J., MURPHY E., NAYLOR B.J., NERI R., NGUYEN H.T., OLIVER S.J., OMONT A., PAGE M.J., PAPAGEORGIOU A., PEARSON C.P., PEREZ-FOURNON I., POHLEN M., RANGWALA N., RAWLINGS J.I., RAYMOND G., RIECHERS D., RODIGHIERO G., ROSEBOOM I.G., ROWAN-ROBINSON M., SCHULZ B., SCOTT D., SCOTT K., SERRA P., SEYMOUR N., SHUPE D.L., SMITH A.J., SYMEONIDIS M., TUGWELL K.E., VACCARI M., VALIANTE E., VALTCHANOV I., VERMA A., VIERO M.P., VIGROUX L., WANG L., WIEBE D., WRIGHT G., XU C.K., ZEIMANN G., ZEMCOV M., ZMUIDZINAS J.
	Astrophys. J., 732L, 35 (2011)
	Discovery of a multiply lensed submillimeter galaxy in early HerMES Herschel/SPIRE data.
o	Text: <[CCV2011] HLSW-01> N=1. Fig. 1: <[CCV2011] HLSW-01 N> (Nos 1-4).
Ref:	=2011ApJ...738..125G
by	GAVAZZI R. , COORAY A., CONLEY A., AGUIRRE J.E., AMBLARD A., AULD R., BEELEN A., BLAIN A., BLUNDELL R., BOCK J., BRADFORD C.M., BRIDGE C., BRISBIN D., BURGARELLA D., CHANIAL P., CHAPIN E., CHRISTOPHER N., CLEMENTS D.L., COX P., DJORGOVSKI S.G., DOWELL C.D., EALES S., EARLE L., ELLSWORTH-BOWERS T.P., FARRAH D., FRANCESCHINI A., FU H., GLENN J., GONZALEZ SOLARES E.A., GRIFFIN M., GURWELL M.A., HALPERN M., IBAR E., IVISON R.J., JARVIS M., KAMENETZKY J., KIM S., KRIPS M., LEVENSON L., LUPU R., MAHABAL A., MALONEY P.D., MARASTON C., MARCHETTI L., MARSDEN G., MATSUHARA H., MORTIER A.M.J., MURPHY E., NAYLOR B.J., NERI R., NGUYEN H.T., OLIVER S.J., OMONT A., PAGE M.J., PAPAGEORGIOU A., PEARSON C.P., PEREZ-FOURNON I., POHLEN M., RANGWALA N., RAWLINGS J.I., RAYMOND G., RIECHERS D., RODIGHIERO G., ROSEBOOM I.G., ROWAN-ROBINSON M., SCHULZ B., SCOTT D., SCOTT K.S., SERRA P., SEYMOUR N., SHUPE D.L., SMITH A.J., SYMEONIDIS M., TUGWELL K.E., VACCARI M., VALIANTE E., VALTCHANOV I., VERMA A., VIEIRA J.D., VIGROUX L., WANG L., WARDLOW J., WIEBE D., WRIGHT G., XU C.K., ZEIMANN G., ZEMCOV M., ZMUIDZINAS J.
	Astrophys. J., 738, 125 (2011)
	Modeling of the HerMES submillimeter source lensed by a dark matter dominated foreground group of galaxies.
o	Fig. 1: <[GCC2011] GN> (Nos G1-G5), <[CCV2011] HLSW-01 Na> (Nos 1a-1b) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCW2011]
[CCW2011]	(Chen+Cowie+Wang+, 2011)
Write:	<<[CCW2011] A2390-3a>>
N:	2
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SMA 870mu.m observations of the field of ACO 2390.
Ref:	=2011ApJ...733...64C
by	CHEN C.-C. , COWIE L.L., WANG W.-H., BARGER A.J., WILLIAMS J.P.
	Astrophys. J., 733, 64 (2011)
	Submillimeter sources behind the massive lensing clusters A370 and A2390.
o	Fig. 2, Table 2: <[CCW2011] A2390-3a> (Nos a-b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCW2014]
[CCW2014]	(Cooray+Calanog+Wardlow+, 2014)
Write:	<<[CCW2014] GN>> <<[CCW2014] RN>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Note:	HST ACS and WFC3 and Keck NIRC2 observations of the starbursting galaxy HFLS3 at z=6.34.
Ref:	=2014ApJ...790...40C
by	COORAY A. , CALANOG J., WARDLOW J.L., BOCK J., BRIDGE C., BURGARELLA D., BUSSMANN R.S., CASEY C.M., CLEMENTS D., CONLEY A., FARRAH D., FU H., GAVAZZI R., IVISON R.J., LA PORTE N., LO FARO B., MA B., MAGDIS G., OLIVER S.J., OSAGE W.A., PEREZ-FOURNON I., RIECHERS D., RIGOPOULOU D., SCOTT D., VIERO M., WATSON D.
	Astrophys. J., 790, 40 (2014)
	HerMES: the rest-frame UV emission and a lensing model for the z = 6.34 luminous dusty starburst galaxy HFLS3.
o	Table 1: <[CCW2014] GN> (Nos G1-G2), <[CCW2014] RN> (No R1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCW2015]
[CCW2015]	(Coppejans+Cseh+Williams+, 2015)
Write:	<<[CCW2015] JHHMMSS+DDMMSSa>>
N:	1706+16
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA 324.5MHz observations of N=1706 sources in the Bootes field. Note that the format is based on rounded coordinates (rather than truncated). Small letters indicate Gaussian components of the source.
in source:	NAME Bootes Field
Ref:	=2015MNRAS.450.1477C
by	COPPEJANS R. , CSEH D., WILLIAMS W.L., VAN VELZEN S., FALCKE H.
	Mon. Not. R. Astron. Soc., 450, 1477-1485 (2015)
	Megahertz peaked-spectrum sources in the Bootes field I - a route towards finding high-redshift AGN.
o	Table 3: <[CCW2015] JHHMMSS+DDMMSSa> N=1706.
Ref:	=2016MNRAS.459.2455C
by	COPPEJANS R. , CSEH D., VAN VELZEN S., FALCKE H., INTEMA H.T., PARAGI Z., MUELLER C., WILLIAMS W.L., FREY S., GURVITS L.I., KORDING E.G.
	Mon. Not. R. Astron. Soc., 459, 2455-2471 (2016)
	What are the megahertz peaked-spectrum sources?
o	Figs 3-7, Tables 1+5: <[CCW2015] JHHMMSS+DDMMSSa> N=16 added.
=E=	Catalogue in electronic form as J/MNRAS/450/1477
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCW2016]
[CCW2016]	(Chiti+Chatterjee+Wharton+, 2016)
Write:	<<[CCW2016] RT YYMMDD>>
N:	16
Object:	Radio Transient (SIMBAD class: Radio = Radio Source)
Note:	N=16 radio transient events in archival VLA observations of the Galactic Center.
in source:	NAME Galactic Center
Ref:	=2016ApJ...833...11C
by	CHITI A. , CHATTERJEE S., WHARTON R., CORDES J., LAZIO T.J.W., KAPLAN D.L., BOWER G.C., CROFT S.
	Astrophys. J., 833, 11-11 (2016)
	Transient events in archival Very Large Array observations of the Galactic Center.
o	Table 3: <[CCW2016] RT YYMMDD> N=16.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CCZ2022]
[CCZ2022]	(Cooper+Casey+Zavala+, 2022)
Write:	<<[CCZ2022] SSA.NNN7.N>>
N:	2
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 4 (2mm) observations of N=2 mm component of S2CLS SSA22.0007.
in source:	SSA 22
Ref:	=2022ApJ...930...32C
by	COOPER O.R. , CASEY C.M., ZAVALA J.A., CHAMPAGNE J.B., DA CUNHA E., LONG A.S., SPILKER J.S., STAGUHN J.
	Astrophys. J., 930, 32-32 (2022)
	Searching Far and Long. I. Pilot ALMA 2 mm Follow-up of Bright Dusty Galaxies as a Redshift Filter.
o	Tables 1-2: <[CCZ2022] SSA.0007.N> (Nos 1-2).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: CD
CD	(Cordoba obs., Durchmusterung)= CDM = CoD = DM
Write:	<<CD +DD NNNNNA>>
N:	about 515000
Object:	* (SIMBAD class: Star)
Ref:	=1892RNAO...16....1T
by	THOME J.M.
	Results of National Argentine Obs., 16, 1-604 (1892)
	Cordoba Durchmusterung declination -22 to -32.
o	<CD +DD NNNNNA> N=179800.
Ref:	=1894RNAO...17....1T
by	THOME J.M.
	Results of National Argentine Obs., 17, 1-538 (1894)
	Cordoba Durchmusterung declination -32 to -42.
o	<CD +DD NNNNNA> N=160415.
Ref:	=1900RNAO...18....1T
by	THOME J.M.
	Results of National Argentine Obs., 18, 1-502 (1900)
	Cordoba Durchmusterung declination -42 to -52.
o	<CD +DD NNNNNA> N=149447.
Ref:	=1914RNAO...21....1T
by	THOME J.M.
	Results of National Argentine Obs., 21, 1-305 (1914)
	Cordoba Durchmusterung declination -52 to -62.
o	<CD +DD NNNNNA> N=about 18000.
Ref:	=1932RNAO...21....1P
by	PERRINE C.D.
	Results of National Argentine Obs., 21, 1-140 (1932)
	Cordoba Durchmusterung declination -62 to -90.
o	<CD +DD NNNNNA> N=about 7800.
=E=	Catalogue in electronic form as I/114
Details on Acronym: [CD2008]
[CD2008]	(Cabalerro+Dinis, 2008) (Not yet in Simbad)
Write:	<<[CD2008] R>>
N:	25
Object:	Agglomerate (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Study of the spatial structure of regions rich in Hipparcos stars with B(T)-V(T) colours. See also Escorial.
Ref:	=2008AN....329..801C
by	CABALLERO J.A. , DINIS L.
	AN, 329, 801-834 (2008)
	A revisit to agglomerate of early-type Hipparcos stars.
o	Table 1: <Escorial NN> (Nos 1-35). Table 3: <[CD2008] R> (Nos I to XXI).
=E=	Catalogue in electronic form as J/AN/329/801
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CD83]
[CD83]	(Cox+Deharveng, 1983)
Write:	<<[CD83] Shell N>>
N:	5
Object:	Shell (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
in source:	Magellanic Clouds:LMC:30 Dor Nebula = 30 Dor Nebula
Ref:	=1983A&A...117..265C
by	COX P. , DEHARVENG L.
	Astron. Astrophys., 117, 265-271 (1983)
	The morphology and dynamics of the halo of the 30 Doradus nebula.
o	Table 2, Fig.1: <[CD83] Shell N> (Nos 1-3).
Ref:	=1991ApJ...370..541W
by	WANG Q. , HELFAND D.J.
	Astrophys. J., 370, 541-550 (1991)
	An X-ray image of the violent interstellar medium in 30 Doradus.
o	Table 1: Objects are WHHW in SIMBAD. (WH superseded by WHHW). WHHW 0539.4-6860 = WHHW 0539.4-6859
o	Table 2: <[CD83] Shell N> (Nos 4-5) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDA2017]
[CDA2017]	(Caputi+Deshmukh+Ashby+, 2017)
Write:	<<[CDA2017] SM2 NNNNNN>> <<[CDA2017] SM2 NNNNNN>> (not recognised by Simbad, but found in literature)
N:	7
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=7 galaxies at 3.9≤z≤4.9. Use of data from the Spitzer Matching Survey of the UltraVISTA Deep Stripes (SMUVS) survey, and of UltraVISTA data.
Ref:	=2017ApJ...849...45C
by	CAPUTI K.I. , DESHMUKH S., ASHBY M.L.N., COWLEY W.I., BISIGELLO L., FAZIO G.G., FYNBO J.P.U., LE FEVRE O., MILVANG-JENSEN B., ILBERT O.
	Astrophys. J., 849, 45-45 (2017)
	Star formation in galaxies at z ~ 4-5 from the SMUVS Survey: a clear starburst/main-sequence bimodality for Hα emitters on the SFR-M plane.*
o	Table 1: <[CDA2017] SM2 NNNNNN> N=7 among (Nos 103948-104510).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDA2021]
[CDA2021]	(Calvi+Dannerbauer+Arrabal Haro+, 2021)
Write:	<<[CDA2021] PCl-HDF850.1>> <<[CDA2021] PCl-HDF850.1-NN>>
N:	1+23
Object:	Cluster of G + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	GTC OSIRIS spectroscopy of N=1 galaxy protocluster and N=23 confirmed members, in the field of [HDS98] HDF850.1.
in source:	NAME GOODS North Field
Ref:	=2021MNRAS.502.4558C
by	CALVI R. , DANNERBAUER H., ARRABAL HARO P., RODRIGUEZ ESPINOSA J.M., MUNOZ-TUNON C., PEREZ GONZALEZ P.G., GEIER S.
	Mon. Not. R. Astron. Soc., 502, 4558-4575 (2021)
	Probing the existence of a rich galaxy overdensity at z = 5.2.
o	<[CDA2021] PCl-HDF850.1> N=1. Table 3: <[CDA2021] PCl-HDF850.1-NN> (Nos 1-23).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDB2005]
[CDB2005]	(Coleman+Da Costa+Bland-Hawthorn, 2005)= ([CDB2005a])
Write:	<<[CDB2005] FF-N-NNNN>>
N:	152
Object:	* (SIMBAD class: Star)
Note:	Wide-field survey observed at the Siding Spring Observatory 1m telescope and 2dF at the AAT spectroscopic observations of the Sculptor galaxy.
in source:	NAME Scl Dwarf Galaxy
Ref:	=2005AJ....130.1065C
by	COLEMAN M.G. , DA COSTA G.S., BLAND-HAWTHORN J.
	Astron. J., 130, 1065-1082 (2005)
	The absence of extratidal structure in the Sculptor dwarf spheroidal galaxy.
o	Table 7: <[CDB2005] FF-N-NNNN> N=152.
=E=	Catalogue in electronic form as J/AJ/130/1065
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDB2005a]
[CDB2005a]	(Coleman+Da Costa+Bland-Hawthorn, 2005)
*****	Avoid the usage of [CDB2005a], prefer [CDB2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDB2005b]
[CDB2005b]	(Castro-Tirado+De ugarte Postigo+Bihain+, 2005)
Write:	<<[CDB2005b] A>>
N:	2
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	NIR observations at the 1.5m Carlos Sanchez telescope at Tenerife. Detection of two objects in the SWIFT X-ray error box of GRB 051022. Object B is later defined as the host galaxy of the GRB.
Ref:	=2005GCN..4143....1C
by	CASTRO-TIRADO A.J. , DE UGARTE POSTIGO A., BIHAIN G., GUZIY S., PANDEY S.B., JELINEK M., GOROSABEL J.
	GRB Coordinates Network, Circular Service, 4143, 1-None (2005)
	GRB 051022, J & K-band observation.
o	<[CDB2005b] A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDB2017]
[CDB2017]	(Cibinel+Daddi+Bournaud+, 2017) (Not yet in Simbad)
Write:	<<[CDB2017] N>> <<[CDB2017] Ex1>>
N:	6+1
Object:	Clump + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	ALMA CO(5-4) observations of N=6 clumps in UDF 6462, and of N=1 in the field of UDF 6462. Use of HST, Spitzer, Herschel, and VLA data.
in source:	UDF 6462
Ref:	=2017MNRAS.469.4683C
by	CIBINEL A. , DADDI E., BOURNAUD F., SARGENT M.T., LE FLOC'H E., MAGDIS G.E., PANNELLA M., RUJOPAKARN W., JUNEAU S., ZANELLA A., DUC P.-A., OESCH P.A., ELBAZ D., JAGANNATHAN P., NYLAND K., WANG T.
	Mon. Not. R. Astron. Soc., 469, 4683-4704 (2017)
	ALMA constraints on star-forming gas in a prototypical z = 1.5 clumpy galaxy: the dearth of CO(5-4) emission from UV-bright clumps.
o	Fig. 1, Table 2: <[CDB2017] N> (Nos 1-6). Fig. A4, Table B1: <[CDB2017] Ex1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDB2020]
[CDB2020]	(Chartas+Davidson+Brusa+, 2020)
Write:	<<[CDB2020] HS 0810+2554 X>> <<[CDB2020] HS 0810+2554 CN>>
N:	1+9
Object:	(mm) + mm clump (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 3 (100 GHz) and Band 4 (140 GHz) observations of N=1 mm component and N=9 mm clumps in the field of the gravitationally lensed quasar HS 0810+2554.
in source:	[RHB2002] HS 0810+2554
Ref:	=2020MNRAS.496..598C
by	CHARTAS G. , DAVIDSON E., BRUSA M., VIGNALI C., CAPPI M., DADINA M., CRESCI G., PALADINO R., LANZUISI G., COMASTRI A.
	Mon. Not. R. Astron. Soc., 496, 598-611 (2020)
	Linking the small-scale relativistic winds and the large-scale molecular outflows in the z = 1.51 lensed quasar HS 0810+2554.
o	Fig. 1, Table 2: <[CDB2020] HS 0810+2554 X> N=1. Fig. 13, Table 4 : <[CDB2020] HS 0810+2554 CN> (Nos C1-C9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDB98]
[CDB98]	(Cappi+Da Costa+Benoist+, 1998)= (VLG)
Write:	<<[CDB98] NNN>> <<[CDB98] VLG HHMM+DDMM>>
N:	113
Object:	G (SIMBAD class: Galaxy)
Note:	Analysis of Very Luminous Galaxies (VLG) in SSRS2 survey See also table 2: VLGG groups of VLG galaxies. See also [CBD2003].
Ref:	=1998AJ....115.2250C
by	CAPPI A. , DA COSTA L.N., BENOIST C., MAUROGORDATO S., PELLEGRINI P.S.
	Astron. J., 115, 2250-2263 (1998)
	Properties of very luminous galaxies.
o	Table 1: <[CDB98] NNN> (Nos 1-113) = <[CDB98] VLG HHMM+DDMM> N=113. Table 2: <VLGG HHMM+DDMM> N=54.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDC2018]
[CDC2018]	(Champagne+Decarli+Casey+, 2018)
Write:	<<[CDC2018] C-PJDDDa>> <<[CDC2018] C-JHHMMa>>
N:	6+9
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 6 (211-275GHz) observations of N = 15 millimeter sources in the fields of bright quasars.
Ref:	=2018ApJ...867..153C
by	CHAMPAGNE J.B. , DECARLI R., CASEY C.M., VENEMANS B., BANADOS E., WALTER F., BERTOLDI F., FAN X., FARINA E.P., MAZZUCCHELLI C., RIECHERS D.A., STRAUSS M.A., WANG R., YANG Y.
	Astrophys. J., 867, 153-153 (2018)
	No evidence for millimeter continuum source overdensities in the environments of z >= 6 quasars.
o	Fig. 4, Table 2: <[CDC2018] C-PJDDDa> N=6, <[CDC2018] C-JHHMMa> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDD2000]
[CDD2000]	(Casertano+De Mello+Dickinson+, 2000)= ([CDD2000a])
Write:	<<[CDD2000] NNNNN>> <<[CDD2000] HDFS JHHMMSS.ss+DDMMSS.s>>
N:	2656
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	WHST WFPC2 observations of HDFS. 'NNNNN' is the SExtractor identification number. See also HDFS.
in source:	NAME HDFS
Ref:	=2000AJ....120.2747C
by	CASERTANO S. , DE MELLO D.F., DICKINSON M., FERGUSON H.C., FRUCHTER A.S., GONZALEZ-LOPEZLIRA R.A., HEYER I., HOOK R.N., LEVAY Z., LUCAS R.A., MACK J., MAKIDON R.B., MUTCHLER M., SMITH T.E., STIAVELLI M., WIGGS M.S., WILLIAMS R.E.
	Astron. J., 120, 2747-2824 (2000)
	WFPC2 observations of the Hubble Deep Field South.
o	Table 6: <[CDD2000] NNNNN> N=2656 among (Nos 1-10719) = <[CDD2000] HDFS JHHMMSS.ss+DDMMSS.s> N=2656 = <HDFS JHHMMSS.ss+DDMMSS.s> N=2656.
=E=	Catalogue in electronic form as J/AJ/120/2747
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDD2000a]
[CDD2000a]	(Casertano+De Mello+Dickinson+, 2000)
*****	Avoid the usage of [CDD2000a], prefer [CDD2000]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDD2000b]
[CDD2000b]	(Covone+De Ritis+Dominik+, 2000)= AGAPE
Write:	<<[CDD2000b] NN>>
N:	19
Object:	Lensing Event (SIMBAD class: LensingEv = (Micro)Lensing Event)
Note:	AGAPE candidate events toward M 31.
in source:	M 31 = NGC 224
Ref:	=2000A&A...357..816C
by	COVONE G. , DE RITIS R., DOMINIK M., MARINO A.A.
	Astron. Astrophys., 357, 816-822 (2000)
	Detecting planets around stars in nearby galaxies.
o	Table 1: <[CDD2000b] NN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDD2000c]
[CDD2000c]	(Castro+Diercks+Djorgovski+, 2000)
Write:	<<[CDD2000c] GRB 000301C abs N.NNNN>>
N:	1
Object:	Absorber
Note:	Keck II ESI observations. Aborption system in the spectrum of GRB 000301C.
Ref:	=2000GCN...605....1C
by	CASTRO S.M. , DIERCKS A., DJORGOVSKI S.G., KULKARNI S.R., GALAMA T.J., BLOOM J.S., HARRISON F.A., FRAIL D.A.
	GRB Coordinates Network, Circular Service, 605, 1-None (2000)
	GRB 000301C: a precise redshift determination.
o	<[CDD2000c] GRB 000301C abs N.NNNN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDD87]
[CDD87]	(Cristiani+De Souza+D'Odorico+, 1987)
Write:	<<[CDD87] NN>>
N:	44
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	ESO 3.6m telescope OPTOPUS spectroscopic observations of ACO 3532.
in source:	Klem 22 = ACO 3532
Ref:	=1987A&A...179..108C
by	CRISTIANI S. , DE SOUZA R., D'ODORICO S., LUND G., QUINTANA H.
	Astron. Astrophys., 179, 108-114 (1987)
	Radial velocities of galaxies in the cluster Klemola 22 from observations with OPTOPUS, the ESO multiple object spectroscopy facility.
o	Table 1: <[CDD87] NN> (Nos 1-44).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDD99]
[CDD99]	(Cimatti+Daddi+Di Serego Alighieri+, 1999)= (ERG)
Write:	<<[CDD99] JHHMMSS+DDMM.m>>
N:	9
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	NTT SOFI et VLT ISAAC observations.
Ref:	=1999A&A...352L..45C
by	CIMATTI A. , DADDI E., DI SEREGO ALIGHIERI S., POZZETTI L., MANNUCCI F., RENZINI A., OLIVA E., ZAMORANI G., ANDREANI P., ROETTGERING H.J.A.
	Astron. Astrophys., 352, 45-50 (1999)
	New clues on the nature of extremely red galaxies.
o	Table 1: <[CDD99] JHHMMSS+DDMM.m> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CDF
CDF	(Chandra Deep Field)
*****	Avoid the usage of CDF, prefer [SGC2001]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CDF2003]
[CDF2003]	(Cotton+Dallacasa+Fanti+, 2003) (Not yet in Simbad)
Write:	<<[CDF2003] 3C 138 AN>>
N:	3+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Radio components of 3C 138.
in source:	3C 138
Ref:	=2003A&A...406...43C
by	COTTON W.D. , DALLACASA D., FANTI C., FANTI R., FOLEY A.R., SCHILIZZI R.T., SPENCER R.E.
	Astron. Astrophys., 406, 43-50 (2003)
	The Faraday screen near the nucleus of the CSS quasar 3C 138.
o	Figs 2, 3: <[CDF2003] 3C 138 AN> (Nos a-c, b1-b2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDF88]
[CDF88]	(Chavarria-K+De Lara+Finkenzeller+, 1988)
Write:	<<[CDF88] NN>> <<[CDF88] HA NNW>>
N:	17+14+4
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	1988A&A...197..151C: Table 1: (Nos 1-17), R stars associated with the Serpens Cloud Table 6: (Nos HA 1 to HA 14), H-alpha emission stars associated with the Serpens Cloud 1991A&A...243..139D: Table 2: (Nos HA 4N, 4S, 7N, 7S) added See also [DCL91]
in source:	NAME Serpens Cloud
Ref:	=1988A&A...197..151C
by	CHAVARRIA-K. C. , DE LARA E., FINKENZELLER U., MENDOZA E.E., OCEGUEDA J.
	Astron. Astrophys., 197, 151-160 (1988)
	An observational study of the Herbig Ae star VV Serpentis, and of stars with reflection nebula associated with its dark cloud.
o	Table 1: <[CDF88] NN> (Nos 1-17). Table 6: <[CDF88] HA NN> (Nos 1-14).
Ref:	=1991A&A...243..139D
by	DE LARA E. , CHAVARRIA-K C., LOPEZ-MOLINA G.
	Astron. Astrophys., 243, 139-142 (1991)
	Distance to the Serpens cloud. II.
o	Table 2: <[CDF88] HA NNW> (Nos 4N, 4S, 7N, 7S). Table 4: <[DCL91] IRS NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDF99]
[CDF99]	(Clemments+Desert+Franceschini+, 1999)
Write:	<<[CDF99] FN-NNN>>
N:	50
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Faint sources detected with ISO observations, in 4 fields (F1-F4).
Ref:	=1999A&A...346..383C
by	CLEMENTS D.L. , DESERT F.-X., FRANCESCHINI A., REACH W.T., BAKER A.C., DAVIES J.K., CESARSKY C.
	Astron. Astrophys., 346, 383-391 (1999)
	A deep 12 micron survey with ISO.
o	Table 2: <[CDF99] F1-NNN> N=15 among (Nos F1-0 to F1-48), <[CDF99] F2-NNN> N=11 among (Nos F2-0 to F2-195), <[CDF99] F3-NNN> N=10 among (Nos F3-0 to F3-37), <[CDF99] F4-NNN> N=14 among (Nos F4-0 to F4-68).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CDFS
CDFS
*****	Avoid the usage of CDFS, prefer [BIF2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CDFS
CDFS	(Chandra Deep Field South)
*****	Avoid the usage of CDFS, prefer GOODS-MUSIC
Origin	of the Acronym: L (2008A&A...488..463M)
Details on Acronym: CDFS
CDFS	(Chandra Deep Field South)
*****	Avoid the usage of CDFS, prefer [GZW2002]
Origin	of the Acronym: L (2003ApJ...592..721G)
Details on Acronym: CDFS
CDFS	(Chandra Deep Field South)
*****	Avoid the usage of CDFS, prefer K20S
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CDFS-H
CDFS-H	(Chandra Deep Field South H-band survey)
*****	Avoid the usage of CDFS-H, prefer [MBR2003]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CDG2015]
[CDG2015]	(Casewell+Dobbie+Geier+, 2015)
Write:	<<[CDG2015] APWDNN>>
Object:	Poss. WD (SIMBAD class: WhiteDwarf_Candidate = White Dwarf Candidate)
Stat:	is completely incorporated in Simbad
Note:	WHT ISIS optical spectroscopy of N=14 white dwarf candidates in the field of α Persei open star cluster. Use of archival UKIDSS and SuperCOSMOS surveys.
in source:	NAME alf Per Cluster
Ref:	=2015MNRAS.451.4259C
by	CASEWELL S.L. , DOBBIE P.D., GEIER S., LODIEU N., HAMBLY N.C.
	Mon. Not. R. Astron. Soc., 451, 4259-4265 (2015)
	Optical spectroscopy of candidate Alpha Persei white dwarfs.
o	Table 1: <[CDG2015] APWDNN> (Nos 01-14).
Details on Acronym: CDGS
CDGS	(Chandra Deep Group Survey)
Write:	<<CDGS NN>>
N:	62
Object:	Cluster of G + Group of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-I observations of N=62 galaxy groups and clusters at 0.07<z<1.3.
Ref:	=2015MNRAS.447.3723P
by	PASCUT A. , PONMAN T.J.
	Mon. Not. R. Astron. Soc., 447, 3723-3744 (2015)
	The Chandra Deep Group Survey - cool core evolution in groups and clusters of galaxies.
o	Tables 1-2: <CDGS NN> (Nos 1-62).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CDJ2011]
[CDJ2011]	(Clapson+Domainko+Jamrozy+, 2011) (Not yet in Simbad)
Write:	<<[CDJ2011] OstarN>> <<[CDJ2011] YSON>>
N:	2+2
Object:	* + Poss. YSO (SIMBAD class: Star)
Note:	N=2 O-type stars and N=2 candidate YSOs in Terzan 5.
in source:	Cl Terzan 5
Ref:	=2011A&A...532A..47C
by	CLAPSON A.-C. , DOMAINKO W., JAMROZY M., DYRDA M., EGER P.
	Astron. Astrophys., 532A, 47-47 (2011)
	Multi-wavelength environment of the Galactic globular cluster Terzan 5.
o	Figs 3-4: <[CDJ2011] OstarN> (Nos Ostar1-Ostar2), <[CDJ2011] YSON> (Nos YSO1-YSO2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDJ78]
[CDJ78]	(Clark+Doxsey+Jernican+, 1978)
Write:	<<[CDJ78] SMC X-2 Star NA>> <<[CDJ78] SMC X-3 Star N>>
N:	7+2+7
Object:	* (SIMBAD class: Star)
Note:	Stars in the error circle of X SMC X-2 and X SMC X-3.
Ref:	=1978ApJ...221L..37C
by	CLARK G. , DOXSEY R., LI F., JERNIGAN J.G., VAN PARADIJS J.
	Astrophys. J., 221, 37-41 (1978)
	On two new X-ray sources in the SMC and the high luminosities of the Magellanic X-ray sources.
o	Fig.1: <[CDJ78] SMC X-2 Star N> (Nos 1-7), <[CDJ78] SMC X-3 Star N> (Nos 1-7).
Ref:	=1979MNRAS.186p..43M
by	MURDIN P. , MORTON D.C., THOMAS R.M.
	Mon. Not. R. Astron. Soc., 186, part no 16, 43-44 (1979)
	Optical identification of SMC X-2.
o	<[CDJ78] SMC X-2 Star NA> (Nos 5A, 5B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDK2000]
[CDK2000]	(Castro+Djorgovski+Kulkarni+, 2000+)
Write:	<<[CDK2000] GRB 000926 abs N.NNNN>>
N:	1
Object:	Absorber
Note:	Absorption system in the spectra of GRB 000926. See also [FGD2001].
Ref:	=2000GCN...851....1C
by	CASTRO S.M. , DJORGOVSKI S.G., KULKARNI S.R., BLOOM J.S., GALAMA T.J., HARRISON F.A., FRAIL D.A.
	GRB Coordinates Network, Circular Service, 851, 1-None (2000)
	GRB 000926: improved absorber redshift.
o	<[CDK2000] GRB 000926 abs N.NNNN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDK2003]
[CDK2003]	(Chisholm+Dodelson+Kolb, 2003)
Write:	<<[CDK2003] X-NN>> <<[CDK2003] S-NN>>
N:	87+29
Object:	(X) + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	The SDSS and RASS surveys are used to search for black hole candidates. 'X-NN' are X-ray selected remnant black hole candidates. 'S-NN' are Spectroscopically selected remnant black hole candidates.
Ref:	=2003ApJ...596..437C
by	CHISHOLM J.R. , DODELSON S., KOLB E.W.
	Astrophys. J., 596, 437-450 (2003)
	Stellar-mass black holes in the solar neighborhood.
o	Table 2: <[CDK2003] X-NN> (Nos X-01 to X-87). Table 3: <[CDK2003] S-NN> (Nos S-01 to S-29).
=E=	Catalogue in electronic form as J/ApJ/596/437
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDL2004]
[CDL2004]	(Ciardullo+Durrell+Laychak+, 2004)
Write:	<<[CDL2004] NNN>>
N:	152
Object:	Poss. PN (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
Stat:	is completely incorporated in Simbad
Note:	PNs candidates in M 33 observed with the Kitt Peak 4m telescope.
in source:	M 33 = NGC 598
Ref:	=2004ApJ...614..167C
by	CIARDULLO R. , DURRELL P.R., LAYCHAK M.B., HERRMANN K.A., MOODY K., JACOBY G.H., FELDMEIER J.J.
	Astrophys. J., 614, 167-185 (2004)
	The planetary nebula system of M33.
o	Table 2: <[CDL2004] NNN> (Nos 1-152).
=E=	Catalogue in electronic form as J/ApJ/614/167
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CDM
CDM	(Cordoba obs., Durchmusterung)
*****	Avoid the usage of CDM, prefer CD
Details on Acronym: [CDM2001]
[CDM2001]	(Caraveo+De Luca+Mignani+, 2001) (Not yet in Simbad)
Write:	<<[CDM2001] NN>>
N:	26
Object:	* (SIMBAD class: Star)
Note:	HST WFPC2 observations. N=26 reference stars in the field of Vela PSR.
Ref:	=2001ApJ...561..930C
by	CARAVEO P.A. , DE LUCA A., MIGNANI R.P., BIGNAMI G.F.
	Astrophys. J., 561, 930-937 (2001)
	The distance to the Vela pulsar gauged with Hubble space telescope parallax observations.
o	Fig.2: <[CDM2001] NN> (Nos 1-26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDM2004]
[CDM2004]	(Caputi+Dunlop+McLure+, 2004)
Write:	<<[CDM2004] NNNNN>>
N:	25+1663
Object:	G (SIMBAD class: Galaxy)
Note:	Search for Extremely Red Galaxies from the GOODS HST-ACS surveys, in the GOODS South Field. See also [MCC2004].
in source:	NAME GOODS South Field
Ref:	=2004MNRAS.353...30C
by	CAPUTI K.I. , DUNLOP J.S., McLURE R.J., ROCHE N.D.
	Mon. Not. R. Astron. Soc., 353, 30-42 (2004)
	A deeper view of extremely red galaxies: the redshift distribution in the GOODS/CDFS ISAAC field.
o	Tables 1 to 4: <[CDM2004] NNNN> N=12+3+8+2.
Ref:	=2005MNRAS.361..607C
by	CAPUTI K.I. , DUNLOP J.S., McLURE R.J., ROCHE N.D.
	Mon. Not. R. Astron. Soc., 361, 607-622 (2005)
	The evolution of K_{s}-selected galaxies in the GOODS/CDFS deep ISAAC field.
o	Table 1: <[CDM2004] NNNNN> N=1663.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDM2005]
[CDM2005]	(Coenda+Donzelli+Muriel+, 2005)
Write:	<<[CDM2005] ACO NNNN JHHMMSS.ss+DDMMSS.ss>>
N:	507
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Southern Abell clusters Redshift Survey (SARS): CCD images of 14 ACO clusters.
Ref:	=2005AJ....129.1237C
by	COENDA V. , DONZELLI C.J., MURIEL H., QUINTANA H., INFANTE L., LAMBAS D.G.
	Astron. J., 129, 1237-1248 (2005)
	Photometric observations of southern Abell clusters redshifts survey clusters: galaxy luminosity profiles.
o	Table 1: coordinates of ACO 2799 are 1950 coordinates, not 2000.
o	Table 3: <[CDM2005] ACO NNNN JHHMMSS.ss+DDMMSS.ss> N=507.
=E=	Catalogue in electronic form as J/AJ/129/1237
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDM2012]
[CDM2012]	(Caputi+Dunlop+McLure+, 2012)
Write:	<<[CDM2012] NNNNN>>
N:	25
Object:	G (SIMBAD class: Galaxy)
Note:	N=25 extremely red galaxies in the UKIDSS Ultra-Deep Survey field. Use of 4.5µm data from the Spitzer SEDS survey and deep H-band data from the HST CANDELS survey.
Ref:	=2012ApJ...750L..20C
by	CAPUTI K.I. , DUNLOP J.S., McLURE R.J., HUANG J.-S., FAZIO G.G., ASHBY M.L.N., CASTELLANO M., FONTANA A., CIRASUOLO M., ALMAINI O., BELL E.F., DICKINSON M., DONLEY J.L., FABER S.M., FERGUSON H.C., GIAVALISCO M., GROGIN N.A., KOCEVSKI D.D., KOEKEMOER A.M., KOO D.C., LAI K., NEWMAN J.A., SOMERVILLE R.S.
	Astrophys. J., 750L, 20 (2012)
	The nature of extremely red H - [4.5] > 4 galaxies revealed with SEDS and CANDELS.
o	Table : <[CDM2012] NNNNN> N=25 among (Nos 25215-38833).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CDN
CDN	(Comparison Dark Nebula)
N:	1
Object:	Bright-Dark Nebula (SIMBAD class: DarkNeb = Dark Cloud (nebula))
Ref:	=1974A&A....32..465F
by	FITZGERALD M.P.
	Astron. Astrophys., 32, 465-474 (1974)
	A remarkable "Bright Dark Nebula" in Chamaeleon.
o	<NAME BDN> <NAME CDN>
Details on Acronym: [CDP2010]
[CDP2010]	(Christensen+D'Odorico+Pettini+, 2010)
Write:	<<[CDP2010] LN>> <<[CDP2010] imN>>
N:	2+4
Object:	Grav. lens + Grav. lensed image of a G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	VLT X-Shooter observations of the gravitational lens system CSWA 5. See also CSWA.
in source:	CSWA 5
Ref:	=2010MNRAS.406.2616C
by	CHRISTENSEN L. , D'ODORICO S., PETTINI M., BELOKUROV V., EVANS N.W., KELLOGG M., VERNET J.
	Mon. Not. R. Astron. Soc., 406, 2616-2626 (2010)
	X-shooter observations of the gravitational lens system CASSOWARY 5.
o	<CSWA NN> (No. 5). Fig. 1, Table 1: <[CDP2010] LN> (Nos L1-L2), <[CDP2010] imN> (Nos im1-im4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CDS
CDS	(Centre de Donnees de Strasbourg)= (W) = (Wack) = (Wackerling)
Write:	<<*Em CDS** NNNN>>
N:	5326
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Ref:	=1970MmRAS..73..153W
by	WACKERLING L.R.
	Mem. R. Astron. Soc., 73, 153-319 (1970)
	A catalogue of early-type stars whose spectra have shown emission lines.
o	<Em* CDS NNNN> (Nos 1-5326).
=E=	Catalogue in electronic form as III/17
=E=	Catalogue in electronic form as <III/17B/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDS2003]
[CDS2003]	(Cannon+Dohm-Palmer+Skillman+, 2003)
Write:	<<[CDS2003] NGC 625 A>> <<[CDS2003] NGC 625 H-beta N>>
N:	4+2
Object:	HII + H-beta (SIMBAD class: Region = Region defined in the Sky)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of NGC 625. N=4 bright HII regions (Nos A-D). [CDS2003] NGC 625 A, B, C are the optical counterparts of [CS2004b] A, B, C, but not D. N=2 areas of high H-beta equivalent width.
in source:	NGC 625
Ref:	=2003AJ....126.2806C
by	CANNON J.M. , DOHM-PALMER R.C., SKILLMAN E.D., BOMANS D.J., COTE S., MILLER B.W.
	Astron. J., 126, 2806-2830 (2003)
	The recent evolution of the dwarf starburst galaxy NGC 625 from Hubble Space Telescope imaging.
o	Fig.3, Table 4: <[CDS2003] NGC 625 A> (Nos A-D). Fig.3, Table 5: <[CDS2003] NGC 625 H-β N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDS2009]
[CDS2009]	(Cote+Draginda+Skillman+, 2009)
Write:	<<[CDS2009] ESO NNN-GNNN NN>> <<[CDS2009] DDO 161 NN>> <<[CDS2009] Centaurus 6 N>> <<[CDS2009] UGCA 365 N>> <<[CDS2009] IC 4316 N>> <<[CDS2009] UKS 1424-460 N>> <<[CDS2009] NGC NNNN NN>>
N:	282
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	CTIO 0.9m telescope Halpha narrow-band imaging of 17 dwarf irregular galaxies in the Centaurus A Group.
in source:	NAME CEN A GROUP
Ref:	=2009AJ....138.1037C
by	COTE S. , DRAGINDA A., SKILLMAN E.D., MILLER B.W.
	Astron. J., 138, 1037-1061 (2009)
	Star formation in dwarf galaxies of the nearby Centaurus A Group.
o	Table 3: <[CDS2009] ESO NNN-GNNN NN> N=15+5+5+8+29+5+10+40+34, <[CDS2009] NGC NNNN NN> N=6+17+63, <[CDS2009] DDO 161 NN> (Nos 1-34), <[CDS2009] Centaurus 6 N> (Nos 1-4), <[CDS2009] UGCA 365 N> (No. 1), <[CDS2009] IC 4316 N> (Nos 1-5), <[CDS2009] UKS 1424-460 N> (No. 1).
=E=	Catalogue in electronic form as <J/AJ/138/1037/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDS2018]
[CDS2018]	(Cantiello+D'Abrusco+Spavone+, 2018)
Write:	<<[CDS2018] NGC 3115 UCD NN>> <<[CDS2018] NGC 3115 LSB N>> <<[CDS2018] NGC 3115 Interacting N>> <<[CDS2018] NGC 3115 Ring N>> <<[CDS2018] NGC 3115 Lens>>
N:	24+8+4+4+1
Object:	Poss. UCD + Poss. LSB + Poss. IG + G + Le? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT VST observations of N=24 ultra compact dwarf (UCD) candidates, N=8 low surface brightness (LSB) objects, N=4 interacting galaxies, N=4 galaxies with rings and bars, and N=1 strong gravitational lens candidate.
Ref:	=2018A&A...611A..93C
by	CANTIELLO M. , D'ABRUSCO R., SPAVONE M., PAOLILLO M., CAPACCIOLI M., LIMATOLA L., GRADO A., IODICE E., RAIMONDO G., NAPOLITANO N., BLAKESLEE J.P., BROCATO E., FORBES D.A., HILKER M., MIESKE S., PELETIER R., VAN DE VEN G., SCHIPANI P.
	Astron. Astrophys., 611A, 93-93 (2018)
	VEGAS-SSS. II. Comparing the globular cluster systems in NGC 3115 and NGC 1399 using VEGAS and FDS survey data. The quest for a common genetic heritage of globular cluster systems.
o	Table A.1: <[CDS2018] NGC 3115 UCD NN> (Nos 1-24). Figs A.3-A.6, Table A.2: <[CDS2018] NGC 3115 LSB N> (Nos 1-8), <[CDS2018] NGC 3115 Interacting N> (Nos 1-4), <[CDS2018] NGC 3115 Ring N> (Nos 1-4), <[CDS2018] NGC 3115 Lens> N=1.
=E=	Catalogue in electronic form as J/A+A/611/A93
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CDS90
CDS90	(Condon+Dickey+Salpeter, 1990)
Write:	<<CDS90 RNNN>> <<CDS90 RNNNA>> <<CDS90 RNNNn>> <<CDS90 NNN>>
N:	354+130
Object:	(Rad) + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	1st ref.: Table II: Format 'R1' to 'R354', R for Radio-source. Table III: format NNN, N=130 galaxies 2nd ref.: 2 other radio-sources are found near 'CDS90 R147' and 'R202', the authors give them the format 'R147n' and 'R202n'. 'CDS90 R182', 'R203', and 'R307' contain 2 radio-sources, the authors give them the format 'R182A and B', etc...
Ref:	=1990AJ.....99.1071C
by	CONDON J.J. , DICKEY J.M., SALPETER E.E.
	Astron. J., 99, 1071-1078 (1990)
	A 1.4 GHz source survey in an area without nearby rich galaxy clusters.
o	Table II: <CDS90 ANNN> N=354, (Nos R1-R354); Table III: <CDS90 NNN> N=130
Ref:	=1996ApJS..103..331L
by	LU N.Y. , HOFFMAN G.L., SALPETER E.E., HOUCK J.R.
	Astrophys. J., Suppl. Ser., 103, 331-362 (1996)
	Radio properties and optical identification of two samples of millijansky radio sources at 1.4 GHz.
o	<CDS90 RNNNn> (Nos R147n, R202n), <CDS90 RNNNA> (Nos R182A, R182B, R203A, R203B, R307A, R307B) added
=E=	Catalogue in electronic form as J/AJ/99/1071
=E=	Catalogue in electronic form as J/ApJS/103/331
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CDS97]
[CDS97]	(Cunow+Duemmler+Spiekermann+, 1997)
Write:	<<[CDS97] ACO NNNN 1-NN>> <<[CDS97] ACO NNNN 2-NN>> <<[CDS97] ACO NNNN N>> <<[CDS97] ACO S NNN 1-NN>> <<[CDS97] ACO S NNN 2-NN>>
N:	117+162
Object:	G + * in ClG (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Tables: N=117 galaxies + 162 stars in 10 ACO
in source:	ACO 916
in source:	ACO S 645
in source:	ACO 3471
in source:	ACO 3528
in source:	ACO S 726
in source:	ACO 1732
in source:	ACO 3558
in source:	ACO 3576
in source:	ACO 1996
in source:	ACO 3621
Ref:	=1997A&AS..125...71C
by	CUNOW B. , DUEMMLER R., SPIEKERMANN G., UNGRUHE R., WARGAU W.F.
	Astron. Astrophys., Suppl. Ser., 125, 71-73 (1997)
	Photometric CCD sequences for calibration of the ESO/SERC atlas.
o	Tables: <[CDS97] ACO NNNN 1-NN>, <[CDS97] ACO NNNN 2-NN>, <[CDS97] ACO S 1-NN>, <[CDS97] ACO S 2-NN>, <[CDS97] ACO NNNN N>, N=117+162
=E=	Catalogue in electronic form as J/A+AS/125/71
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDS98]
[CDS98]	(Cornett+Dorman+Smith+, 1998)
Write:	<<[CDS98] NN>>
N:	13
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	UIT observations aboard Astro 1 and Astro 2 flights Figs1, 2: Maps, Identif. charts.
in source:	ACO 2246
Ref:	=1998AJ....116...44C
by	CORNETT R.H. , DORMAN B., SMITH E.P., FANELLI M.N., OEGERLE W.R., BOHLIN R.C., NEFF S.G., O'CONNELL R.W., ROBERTS M.S., SMITH A.M., STECHER T.P.
	Astron. J., 116, 44-54 (1998)
	Ultraviolet imaging of the z = 0.23 cluster Abell 2246.
o	Table 3: <[CDS98] NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CDT
CDT	(Castellanos+Diaz+Terlevich)
Write:	<<CDT NGC NNNN N>>
N:	5+4+1
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Giant HII regions in 3 NGC galaxies. See also [VSH98].
in source:	NGC 1232
in source:	NGC 925
in source:	NGC 1637
Ref:	=2002MNRAS.329..315C
by	CASTELLANOS M. , DIAZ A.I., TERLEVICH E.
	Mon. Not. R. Astron. Soc., 329, 315-335 (2002)
	A comprehensive study of reported high-metallicity giant H II regions - I. Detailed abundance analysis.
o	Table 4: <CDT NGC 1232 N> (Nos 1-5). Table 5: <CDT NGC 925 N> (Nos 1-4). Table 6: <CDT NGC 1637 N> (No. 1).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CDT2005]
[CDT2005]	(Chary+Dickinson+Teplitz+, 2005)
Write:	<<[CDT2005] DDD.ddddd+DD.ddddd>>
N:	4
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spitzer MIPS 24 mu observations of SN host galaxies in the GOODS-North and -South fields using Spitzer MIPS data. N=4 host galaxies in Tables 1, 2 which are not already in SIMBAD.
Ref:	=2005ApJ...635.1022C
by	CHARY R. , DICKINSON M.E., TEPLITZ H.I., POPE A., RAVINDRANATH S.
	Astrophys. J., 635, 1022-1030 (2005)
	Dust in the host galaxies of supernovae.
o	Tables 1, 2: <[CDT2005] DDD.ddddd+DD.ddddd> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDT2019]
[CDT2019]	(Comeron+Djupvik+Torra+, 2019)
Write:	<<[CDT2019] JHHMMSS.ss+DDMMSS.s>>
N:	21
Object:	Poss. OB* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Calar Alto 2.2m telescope PANIC NIR observations of N=21 OB star candidates in the RAFGL 5475 association.
in source:	RAFGL 5475
Ref:	=2019A&A...622A.134C
by	COMERON F. , DJUPVIK A.A., TORRA J., SCHNEIDER N., PASQUALI A.
	Astron. Astrophys., 622A, 134-134 (2019)
	A distant OB association around RAFGL 5475.
o	Fig. 7, Table 2: <[CDT2019] JHHMMSS.ss+DDMMSS.s> N=21.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CDZ2003]
[CDZ2003]	(Charlton+Ding+Zonak+, 2003)
Write:	<<[CDZ2003] QSO J1634+7031 abs N.NNNN>>
N:	3
Object:	Absorber
Note:	N=3 absorption systems in the line of sight of PG 1634+706 = QSO J1634+7031.
Ref:	=2003ApJ...589..111C
by	CHARLTON J.C. , DING J., ZONAK S.G., CHURCHILL C.W., BOND N.A., RIGBY J.R.
	Astrophys. J., 589, 111-125 (2003)
	High-resolution STIS/Hubble Space Telescope and HIRES/Keck spectra of three weak Mg II absorbers toward PG 1634+706.
o	Table 2: <[CDZ2003] QSO J1634+7031 abs N.NNNN> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CE
CE	(Calan-ESO survey)
Write:	<<CE NNN>>
N:	542
Object:	PM* (SIMBAD class: HighPM* = High Proper Motion Star)
Stat:	is completely incorporated in Simbad
Note:	Calan-ESO proper-motion catalog of 542 stars.
Ref:	=2001ApJS..133..119R
by	RUIZ M.T. , WISCHNJEWSKY M., ROJO P.M., GONZALEZ L.E.
	Astrophys. J., Suppl. Ser., 133, 119-160 (2001)
	Calan-ESO proper-motion catalog.
o	Table 2: <CE NNN> (Nos 1-542).
=E=	Catalogue in electronic form as J/ApJS/133/119
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Ce
Ce	(Centaurus)
*****	Avoid the usage of Ce, prefer [MM87]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CEB2007]
[CEB2007]	(Clark+Eikenberry+Brandl+, 2007)
Write:	<<[CEB2007] Cluster N>> <<[CEB2007] S.ss-S.ss>>
N:	4+19
Object:	Cluster of * + (IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Wide-field camera on the Palomar 5m telescope and Chandra data (see [ZFR2002]) to search for IR counterparts of X-ray sources in The Antennae.
in source:	NAME the Antennae
Ref:	=2007ApJ...658..319C
by	CLARK D.M. , EIKENBERRY S.S., BRANDL B.R., WILSON J.C., CARSON J.C., HENDERSON C.P., HAYWARD T.L., BARRY D.J., PTAK A.F., COLBERT E.J.M.
	Astrophys. J., 658, 319-327 (2007)
	Infrared counterparts to Chandra X-ray sources in the Antennae.
o	(Erratum) erratum vol. 668, p. 1266 (2007)
o	Table 1: <[CEB2007] Cluster N> (Nos 1-4). Table 3: <[CEB2007] S.ss-S.ss> N=13+6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CEB99]
[CEB99]	(Clements+Eales+Baker, 1999)
Write:	<<[CEB99] WFPC2 NNNN>> <<[CEB99] NICMOS NNN>> <<[CEB99] JHHMMSS.ss+DDMMSS.ss>>
N:	37
Object:	G (SIMBAD class: Galaxy)
Note:	WFPC2, NICMOS/STIS HST observations.
in source:	NAME HDFS
Ref:	=1999MNRAS.308L..11C
by	CLEMENTS D.L. , EALES S.A., BAKER A.C.
	Mon. Not. R. Astron. Soc., 308, 11-16 (1999)
	Candidate high-redshift and primeval galaxies in Hubble Deep Field South.
o	Table 1: <[CEB99] WFPC2 NNNN> N=32 among 2257 = <[CEB99] JHHMMSS.ss+DDMMSS.ss>, <[CEB99] NICMOS NNN> N=5 among N>255 = <[CEB99] JHHMMSS.ss+DDMMSS.ss>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CEC96]
[CEC96]	(Cotera+Erickson+Colgan+, 1996)
Write:	<<[CEC96] NN>> <<[CEC96] A>> <<[CEC96] Source A>>
N:	13+7+2
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=13 * format 'NN', those with emission-line features. N=7 * format 'A', those without significant emission lines Map (Plate 16) See also [CSE99].
in source:	GAL 000.121+00.017
Ref:	=1996ApJ...461..750C
by	COTERA A.S. , ERICKSON E.F., COLGAN S.W.J., SIMPSON J.P., ALLEN D.A., BURTON M.G.
	Astrophys. J., 461, 750-761 (1996)
	The discovery of hot stars near the Galactic center thermal radio filaments.
o	Table 3: HD 1489437 misprint for ???
o	Table 1: <[CEC96] NN> (Nos 1-13), <[CEC96] A> (Nos A-G). Table 3: <[CEC96] Source A> (Nos A-B). <Gal 0.121+0.017>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ced
Ced	(Cederblad)= (Cederblad)
Write:	<<Ced NNNa>>
N:	215
Object:	HII + RFN (SIMBAD class: ISM = Interstellar Medium Object)
Ref:	=1946MeLu2.119....1C
by	CEDERBLAD S.
	Lund Medd. Astron. Obs. Ser. II, 119, 1-166 (1946)
	Studies of bright diffuse galactic nebulae with special regard to their spatial distribution.
o	Catalogue: <Ced NNNa> (Nos 1-215)
=E=	Catalogue in electronic form as VII/231
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CED93]
[CED93]	(Casali+Eiroa+Duncan, 1993)= (CED) = (Serp-SMM) = (Serp-SMM) = (SMM)
Write:	<<[CED93] NNW>>
N:	11+1
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
in source:	NAME Serpens Cloud
Ref:	=1993A&A...275..195C
by	CASALI M.M. , EIROA C., DUNCAN W.D.
	Astron. Astrophys., 275, 195-200 (1993)
	A second phase of star formation in the Serpens core.
o	Authors used the acronym SMM, in Simbad [CED93]
o	<[CED93] N> (Nos 1-6)
Ref:	=1995A&A...298..594W
by	WHITE G.J. , CASALI M.M., EIROA C.
	Astron. Astrophys., 298, 594-605 (1995)
	High resolution molecular line observations of the Serpens Nebula.
o	Fig 1g and text: <[CED93] N> (Nos 7-9) added.
Ref:	=1999ApJS..122..519C
by	CHOI M. , PANIS J.-F., EVANS II N.J.
	Astrophys. J., Suppl. Ser., 122, 519-556 (1999)
	Berkeley-Illinois-Maryland association survey of protostellar collapse candidates in HCO^+ and HCN lines.
o	Fig.2: Sources A, B, C are respectively [JCC87] IRAS 4A, [JCC87] IRAS 4B, and [JCC87] IRAS 4B2, in SIMBAD.
o	Fig.9, Table 3: <[CED93] 4E> N=1 added. Fig.16, Table 3: <[CPE99] IRAS 20050+2720 A> (Nos A-D).
Ref:	=1999MNRAS.309..141D
by	DAVIS C.J. , MATTHEWS H.E., RAY T.P., DENT W.R.F., RICHER J.S.
	Mon. Not. R. Astron. Soc., 309, 141-152 (1999)
	A burst of outflows from the Serpens cloud core: wide-field submillimetre continuum, CO j = 2-1 and optical observations.
o	SMM NN objects are [CED93] NN in SIMBAD.
o	Table 1: <HH NNN> (Nos 456-457). Table 2, Fig.1: <[DMR99] Knot a> (Nos a-c). Fig.1: <[DMR99] Extension N> (Nos 1-2). Fig.4: <[DMR99] Lobe WWaN> N=11. Table 2: <[CED93] NN> (Nos 10-11) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Cederblad
Cederblad	(Cederblad)
*****	Avoid the usage of Cederblad, prefer Ced
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CEERS
CEERS	(Cosmic Evolution Early Release Science Survey)
Write:	<<CEERS JHHMMSS.ss+DDMMSS.s>>
Object:	(NIR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	The Cosmic Evolution Early Release Science Survey (CEERS) is one of 13 JWST early release science (ERS) surveys designed to obtain data covering all areas of astronomy early in Cycle 1. CEERS is based around a mosaic of 10 NIRCam pointings, with six obtaining NIRSpec in parallel and four with MIRI in parallel (four of these pointings also include NIRCam wide-field slitless grism spectroscopy). More information is available at https://ceers.github.io/
Ref:	=2022ApJ...940L..55F
by	FINKELSTEIN S.L. , BAGLEY M.B., ARRABAL HARO P., DICKINSON M., FERGUSON H.C., KARTALTEPE J.S., PAPOVICH C., BURGARELLA D., KOCEVSKI D.D., HUERTAS-COMPANY M., IYER K.G., KOEKEMOER A.M., LARSON R.L., PEREZ-GONZALEZ P.G., ROSE C., TACCHELLA S., WILKINS S.M., CHWOROWSKY K., MEDRANO A., MORALES A.M., SOMERVILLE R.S., YUNG L.Y.A., FONTANA A., GIAVALISCO M., GRAZIAN A., GROGIN N.A., KEWLEY L.J., KIRKPATRICK A., KURCZYNSKI P., LOTZ J.M., PENTERICCI L., PIRZKAL N., RAVINDRANATH S., RYAN R.E.Jr, TRUMP J.R., YANG G., (The CEERS Team), ALMAINI O., AMORIN R.O., ANNUNZIATELLA M., BACKHAUS B.E., BARRO G., BEHROOZI P., BELL E.F., BHATAWDEKAR R., BISIGELLO L., BROMM V., BUAT V., BUITRAGO F., CALABRO A., CASEY C.M., CASTELLANO M., CHAVEZ ORTIZ O.A., CIESLA L., CLERI N.J., COHEN S.H., COLE J.W., COOKE K.C., COOPER M.C., COORAY A.R., COSTANTIN L., COX I.G., CROTON D., DADDI E., DAVE R., DE LA VEGA A., DEKEL A., ELBAZ D., ESTRADA-CARPENTER V., FABER S.M., FERNANDEZ V., FINKELSTEIN K.D., FREUNDLICH J., FUJIMOTO S., GARCIA-ARGUMANEZ A., GARDNER J.P., GAWISER E., GOMEZ-GUIJARRO C., GUO Y., HAMBLIN K., HAMILTON T.S., HATHI N.P., HOLWERDA B.W., HIRSCHMANN M., HUTCHISON T.A., JASKOT A.E., JHA S.W., JOGEE S., JUNEAU S., JUNG I., KASSIN S.A., LE BAIL A., LEUNG G.C.K., LUCAS R.A., MAGNELLI B., MANTHA K.B., MATHARU J., McGRATH E.J., McINTOSH D.H., MERLIN E., MOBASHER B., NEWMAN J.A., NICHOLLS D.C., PANDYA V., RAFELSKI M., RONAYNE K., SANTINI P., SEILLE L.-M., SHAH E.A., SHEN L., SIMONS R.C., SNYDER G.F., STANWAY E.R., STRAUGHN A.N., TEPLITZ H.I., VANDERHOOF B.N., VEGA-FERRERO J., WANG W., WEINER B.J., WILLMER C.N.A., WUYTS S., ZAVALA J.A.
	Astrophys. J., 940L, 55 (2022)
	A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging.
o	<CEERS JHHMMSS.ss+DDMMSS.S> (No. J141946.36+525632.8).
Ref:	=2023ApJ...943L...9Z
by	ZAVALA J.A. , BUAT V., CASEY C.M., FINKELSTEIN S.L., BURGARELLA D., BAGLEY M.B., CIESLA L., DADDI E., DICKINSON M., FERGUSON H.C., FRANCO M., JIMENEZ-ANDRADE E.F., KARTALTEPE J.S., KOEKEMOER A.M., LE BAIL A., MURPHY E.J., PAPOVICH C., TACCHELLA S., WILKINS S.M., ARETXAGA I., BEHROOZI P., CHAMPAGNE J.B., FONTANA A., GIAVALISCO M., GRAZIAN A., GROGIN N.A., KEWLEY L.J., KOCEVSKI D.D., KIRKPATRICK A., LOTZ J.M., PENTERICCI L., PEREZ-GONZALEZ P.G., PIRZKAL N., RAVINDRANATH S., SOMERVILLE R.S., TRUMP J.R., YANG G., YUNG L.Y.A., ALMAINI O., AMORIN R.O., ANNUNZIATELLA M., ARRABAL HARO P., BACKHAUS B.E., BARRO G., BELL E.F., BHATAWDEKAR R., BISIGELLO L., BUITRAGO F., CALABRO A., CASTELLANO M., CHAVEZ ORTIZ O.A., CHWOROWSKY K., CLERI N.J., COHEN S.H., COLE J.W., COOKE K.C., COOPER M.C., COORAY A.R., COSTANTIN L., COX I.G., CROTON D., DAVE R., DE LA VEGA A., DEKEL A., ELBAZ D., ESTRADA-CARPENTER V., FERNANDEZ V., FINKELSTEIN K.D., FREUNDLICH J., FUJIMOTO S., GARCIA-ARGUMANEZ A., GARDNER J.P., GAWISER E., GOMEZ-GUIJARRO C., GUO Y., HAMILTON T.S., HATHI N.P., HOLWERDA B.W., HIRSCHMANN M., HUERTAS-COMPANY M., HUTCHISON T.A., IYER K.G., JASKOT A.E., JHA S.W., JOGEE S., JUNEAU S., JUNG I., KASSIN S.A., KURCZYNSKI P., LARSON R.L., LEUNG G.C.K., LONG A.S., LUCAS R.A., MAGNELLI B., MANTHA K.B., MATHARU J., McGRATH E.J., McINTOSH D.H., MEDRANO A., MERLIN E., MOBASHER B., MORALES A.M., NEWMAN J.A., NICHOLLS D.C., PANDYA V., RAFELSKI M., RONAYNE K., ROSE C., RYAN R.E.Jr, SANTINI P., SEILLE L.-M., SHAH E.A., SHEN L., SIMONS R.C., SNYDER G.F., STANWAY E.R., STRAUGHN A.N., TEPLITZ H.I., VANDERHOOF B.N., VEGA-FERRERO J., WANG W., WEINER B.J., WILLMER C.N.A., WUYTS S., (The CEERS Team)
	Astrophys. J., 943L, 9 (2023)
	Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations.
o	<CEERS JHHMMSS.ss+DDMMSS.s> (No. J141938.19+525613.9).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CEF84]
[CEF84]	(Cudlip+Emerson+Furniss+, 1984)= (FIR)
Write:	<<[CEF84] FIR N>>
N:	7
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	NAME rho Oph Cloud
Ref:	=1984MNRAS.211..563C
by	CUDLIP W. , EMERSON J.P., FURNISS I., GLENCROSS W.M., JENNINGS R.E., KING K.J., LIGHTFOOT J.F., TOWLSON W.A.
	Mon. Not. R. Astron. Soc., 211, 563-573 (1984)
	Far-infrared photometry of the ρ Ophiuchi dark cloud.
o	Table 2: <[CEF84] FIR N> (Nos 1-7)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CEF95]
[CEF95]	(Crawford+Edge+Fabian+, 1995)
Write:	<<[CEF95] HHMMSS.s+DDMMSS>>
N:	48
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Table 1, col.(3,4): G in cluster of galaxies, format 'HHMMSS.s+DDMMSS' See also [AEF92], [CAE99].
Ref:	=1995MNRAS.274...75C
by	CRAWFORD C.S. , EDGE A.C., FABIAN A.C., ALLEN S.W., BOHRINGER H., EBELING H., McMAHON R.G., VOGES W.
	Mon. Not. R. Astron. Soc., 274, 75-84 (1995)
	Optical spectroscopy of the ROSAT X-ray brightest clusters. II.
o	Table 1, col.(3,4): <[CEF95] HHMMSS.s+DDMMSS> N=48
=E=	Catalogue in electronic form as J/MNRAS/274/75
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CEG83]
[CEG83]	(Couch+Ellis+Godwin+, 1983)
Write:	<<[CEG83] A1942 NN>> <<[CEG83] A1525 NN>> <<[CEG83] AC103 NNN>>
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Plate 1a: G in ACO 1942, format 'A1942 NN' Plate 1b: G in ACO 1525, format 'A1525 NN' Plate 1c: G in ACCG 103, format 'AC103 NNN' See also CN.
in source:	ACO 1942
in source:	ACO 1525
in source:	ACCG 103 = ACO S 910
Ref:	=1983MNRAS.205.1287C
by	COUCH W.J. , ELLIS R.S., GODWIN J., CARTER D.
	Mon. Not. R. Astron. Soc., 205, 1287-1312 (1983)
	Spectral energy distributions for galaxies in high redshift clusters - I. Methods and application to three clusters with 0.22 < z < 0.31.
o	Plates 1a, 1b, 1c: <[CEG83] A1942 NN> = <CN A1942 NN> Nos among (Nos 1-81), <[CEG83] A1525 NN> = <CN A1525 NN> Nos among (Nos 1-62), <[CEG83] AC103 NNN> = <CN AC103 NNN> Nos among (Nos 1-145).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CeGi
CeGi	(Cesco+Gibson)
*****	Avoid the usage of CeGi, prefer Y-C
Details on Acronym: [CEH77]
[CEH77]	(Chini+Elsasser+Helefe+, 1977)
Write:	<<[CEH77] NN>>
N:	26
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
in source:	NAME rho Oph Cloud
Ref:	=1977A&A....56..323C
by	CHINI R. , ELSAESSER H., HELEFE H., WEINBERGER R.
	Astron. Astrophys., 56, 323-325 (1977)
	On the infrared sources in the Ophiuchus dark cloud region.
o	<[CEH77] NN> N=26
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Cel
Cel	(Celescope catalog)= (UV)
Write:	<<CEL NNNN>>
N:	5759
Object:	UV Obj. (SIMBAD class: UV = UV-emission Source)
Ref:	=1973SAOSR.350....1D
by	DAVIS R.J. , DEUTSCHMAN W.A., HARAMUNDANIS K.L.
	SAO Special Report, 350, 1-None (1973)
	Celescope catalogue of ultraviolet magnitudes.
o	Catalog: <Cel NNNN> (Nos 1-5759).
=E=	Catalogue in electronic form as <II/6/>
Details on Acronym: [CEM88]
[CEM88]	(Carballo+Eiroa+Mampaso, 1988) (Not yet in Simbad)
Write:	<<[CEM88] GGD NN IRS N>> <<[CEM88] GGD 16-17 IRS N>>
N:	12
Object:	(NIR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	1.55m Carlos Sanchez telescope of the Observatorio del Teide (Tenerife) and 1.23m telescope of the Observatorio de Calar Alto (Almeria) NIR observations of areas containing GGD objects.
Ref:	=1988MNRAS.232..497C
by	CARBALLO R. , EIROA C., MAMPASO A.
	Mon. Not. R. Astron. Soc., 232, 497-505 (1988)
	Near-infrared observations of GGD objects.
o	(Erratum) + erratum vol 235, 543
o	Plate 1: <GGD NNa> (Nos 4a-4b, 10a-10c) added. Plate 1, Table 2: <[CEM88] GGD NN IRS N>, <[CEM88] GGD 16-17 IRS N>, N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CEM91]
[CEM91]	(Couch+Ellis+Malin+, 1991)
====>	Equivalent to: CEMM
Origin	of the Acronym: L (1997MNRAS.291..353B)
Details on Acronym: [CEM91]
[CEM91]	(Couch+Ellis+Malin+, 1991)
====>	Equivalent to: CEMM
Origin	of the Acronym: L (1997MNRAS.291..353B)
Details on Acronym: CEMM
CEMM	(Couch+Ellis+Malin+Maclaren)= [CEM91]
Write:	<<CEMM ANNNN.NNAAA>> <<CEMM ANNNN.NN/NNAA>> <<CEMM ANNNN.NNAA/AA>>
N:	111
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	Format: the first part 'ANNNN' is an internal numbering of sequential plates. The second part is an internal designation of each cluster on a plate.
Ref:	=1991MNRAS.249..606C
by	COUCH W.J. , ELLIS R.S., MALIN D.F., MacLAREN I.
	Mon. Not. R. Astron. Soc., 249, 606-628 (1991)
	A uniformly selected catalogue of distant galaxy clusters.
o	Table 3: <CEMM ANNNN.NNAAA>, <CEMM ANNNN.NN/NNAA>, <CEMM ANNNN.NNAA/AA> N=111. Table 6: <CEMM ANNNN.NNAA a>, <CEMM ANNNN.NNAA a+a>, <CEMM ANNNN.N/NNA a>, <CEMM ANNNN.NNAA NN> N=94.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CEMM
CEMM	(Couch+Ellis+Malin+Maclaren)= [CEM91]
Write:	<<CEMM ANNNN.NNAA a>> <<CEMM ANNNN.NNAA a+a>> <<CEMM ANNNN.N/NNA a>> <<CEMM ANNNN.NNAA NN>>
N:	94
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Galaxies in CEMM clusters. A letter 'a' or a number 'NN' is added at the cluster format, to designate the galaxy in the cluster.
Ref:	=1991MNRAS.249..606C
by	COUCH W.J. , ELLIS R.S., MALIN D.F., MacLAREN I.
	Mon. Not. R. Astron. Soc., 249, 606-628 (1991)
	A uniformly selected catalogue of distant galaxy clusters.
o	Table 3: <CEMM ANNNN.NNAAA>, <CEMM ANNNN.NN/NNAA>, <CEMM ANNNN.NNAA/AA> N=111. Table 6: <CEMM ANNNN.NNAA a>, <CEMM ANNNN.NNAA a+a>, <CEMM ANNNN.N/NNA a>, <CEMM ANNNN.NNAA NN> N=94.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Cen
Cen	(Centaurus)
*****	Avoid the usage of Cen, prefer [ABC89]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cen
Cen	(Cen A group)
*****	Avoid the usage of Cen, prefer [CFC97]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cen
Cen	(Centaurus)
Write:	<<NAME Cen NN>>
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	Centaurus cluster of galaxies is composed of two velocity components, 'Cen 30' (mean velocity 3000kms-1), and 'Cen 45' (mean velocity 4500kms-1).
in source:	Centaurus Cluster = ACO 3526
Ref:	=1986MNRAS.221..453L
by	LUCEY J.R. , CURRIE M.J., DICKENS R.J.
	Mon. Not. R. Astron. Soc., 221, 453-472 (1986)
	The Centaurus cluster of galaxies - II. The bimodal velocity structure.
o	<NAME CEN 30> <NAME CEN 45>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CEN77]
[CEN77]	(Cooke+Emerson+Nandy+, 1977)
Write:	<<[CEN77] NN>>
N:	29
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Ref:	=1977MNRAS.178..687C
by	COOKE J.A. , EMERSON D., NANDY K., REDDISH V.C., SMITH M.G.
	Mon. Not. R. Astron. Soc., 178, 687-691 (1977)
	Radial velocities of faint galaxies from objective prism plates.
o	Table 1: <[CEN77] NN> (Nos 1-29).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CENSORS
CENSORS	(Combined EIS-NVSS Survey Of Radio Sources)
Write:	<<CENSORS NNN>> <<CENSORS XN>> <<CENSORS DN>>
N:	150+3+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	New sample of radio-sources designated CENSORS. CENSORS has been defined by combining the NVSS and the EIS survey. (Nos 1-150) include only those NVSS sources which are real and fall within the EIS Patch D, 3 sources (Nos X1-X3) not targeted in the original EISD radio observations are added, and (No. D1) one pair of 2 NVSS sources. See also EISD.
Ref:	=2003MNRAS.346..627B
by	BEST P.N. , ARTS J.N., ROETTGERING H.J.A., RENGELINK R., BROOKES M.H., WALL J.
	Mon. Not. R. Astron. Soc., 346, 627-683 (2003)
	CENSORS: A Combined EIS-NVSS Survey Of Radio Sources - I. Sample definition, radio data and optical identifications.
o	Table A1: <EISD NNN> (Nos 1-199). Table C1: <CENSORS NNN> (Nos 1-150), <CENSORS XN> (Nos X1-X3), <CENSORS D1> N=1.
=E=	Catalogue in electronic form as J/MNRAS/346/627
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Century
Century	(Century survey)
*****	Avoid the usage of Century, prefer [GG99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: cep
cep	(Cepheus)
*****	Avoid the usage of cep, prefer [ABC90]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cep
Cep	(Cepheus)
*****	Avoid the usage of Cep, prefer [MWC53]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CEP2007]
[CEP2007]	(Chiar+Ennico+Pendleton+, 2007)
Write:	<<[CEP2007] QNN-N>> <<[CEP2007] Velucores N-N>> <<[CEP2007] Quidust NN-N>> (not recognised by Simbad, but found in literature)
N:	16+4
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRS observations of field stars located behind dense clouds.
Ref:	=2007ApJ...666L..73C
by	CHIAR J.E. , ENNICO K., PENDLETON Y.J., BOOGERT A.C.A., GREENE T., KNEZ C., LADA C., ROELLIG T., TIELENS A.G.G.M., WERNER M., WHITTET D.C.B.
	Astrophys. J., 666L, 73-76 (2007)
	The relationship between the optical depth of the 9.7 µm silicate absorption feature and infrared differential extinction in dense clouds.
o	Table 1: <[CEP2007] Q NN-N> N=16, <[CEP2007] Velucores N-N> (Nos 1-1 to 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CER2013]
[CER2013]	(Clark+Eikenberry+Raines+, 2013) (Not yet in Simbad)
Write:	<<[CER2013] A>>
N:	2
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	KPNO 4m telescope FISICA NIR spectroscopy of the central regions of NGC 1569.
in source:	NGC 1569
Ref:	=2013MNRAS.428.2290C
by	CLARK D.M. , EIKENBERRY S.S., RAINES S.N., GRUEL N., ELSTON R., GUZMAN R., BOREMAN G., GLENN P.E.
	Mon. Not. R. Astron. Soc., 428, 2290-2294 (2013)
	Probing the super star cluster environment of NGC 1569 using FISICA.
o	Fig. 2: <[CER2013] Region A> (Nos C-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CES2009]
[CES2009]	(Currie+Evans+Spitzbart+, 2009)
Write:	<<[CES2009] NNN>>
N:	165
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS observations of h Persei.
in source:	h Per Cluster = NGC 869
Ref:	=2009AJ....137.3210C
by	CURRIE T. , EVANS N.R., SPITZBART B.D., IRWIN J., WOLK S.J., HERNANDEZ J., KENYON S.J., PASACHOFF J.M.
	Astron. J., 137, 3210-3221 (2009)
	The X-ray environment during the epoch of terrestrial planet formation: Chandra observations of h Persei.
o	Tables 1-2: <[CES2009] NNN> N=165 among (Nos 1-330).
=E=	Catalogue in electronic form as J/AJ/137/3210
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Cet
Cet	(Cetus)
*****	Avoid the usage of Cet, prefer [SDM2004]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CF
CF	(Control Field)
*****	Avoid the usage of CF, prefer [AS82]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CF
CF	(Cape obs., Faint *)= CFS
Write:	<<CF NNNNN>>
N:	20554
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1939CF....C......0S
by	SPENCER JONES H. , JACKSON J.
	Royal Obs. Cape of Good Hope. London (on magnetic tape), 0-None (1939)
	Catalogue of 20554 faint stars in the Cape astrographic zone -40 to -52 for the equinox of 1900.0, Royal Obs. Cape of Good Hope.
o	<CF NNNNN> (Nos 1-20554).
=E=	Catalogue in electronic form as I/6
Details on Acronym: Cf
Cf	(Cancer cl., faint)
*****	Avoid the usage of Cf, prefer [CSD91]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CF2008]
[CF2008]	(Crowther+Fyrness, 2008)
Write:	<<[CF2008] NWW>>
N:	3+2
Object:	(Near IR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Stat:	is completely incorporated in Simbad
Note:	UKIRT UFTI, Steward 2.3m telescope IRCam, and VLT ISAAC observations of the HII region [WWB83] 023.96+0.15.
in source:	[WWB83] G023.96+0.15
Ref:	=2008A&A...492..111C
by	CROWTHER P.A. , FURNESS J.P.
	Astron. Astrophys., 492, 111-115 (2008)
	On the central ionizing star of G23.96+0.15 and near-IR spectral classification of O stars.
o	Paragraph 1. IRAS 8434-0242 is a misprint for IRAS 18434-0242.
o	Fig.1, Table 1: <[CF2008] NWW> (Nos 1-3, 3NW, 3SE).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CF2019]
[CF2019]	(Chiti+Frebel, 2019)
Write:	<<[CF2019] Sgr-NN>>
N:	4
Object:	Giant * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Magellan Baade telescope MagE spectroscopic observations of N=4 stars in the Sagittarius dwarf galaxy. See also [HEM2018] NNNNNNN.
in source:	NAME SDG = NAME Sgr Dwarf Galaxy
Ref:	=2019ApJ...875..112C
by	CHITI A. , FREBEL A.
	Astrophys. J., 875, 112-112 (2019)
	Four metal-poor stars in the Sagittarius dwarf spheroidal galaxy.
o	Table 1: <[CF2019] Sgr-NN> N=4 among (Nos 2-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CF77]
[CF77]	(Cohen+Frogel, 1977)= ([CF77a])
Write:	<<[CF77] Mon R2 N>> <<[CF77] Mon R2 Star B>> <<[CF77] OMC 2 N>>
N:	6+3
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	NAME Mon R2 GMC
in source:	OMC:OMC 2 = OMC 2
Ref:	=1977ApJ...211..178C
by	COHEN J.G. , FROGEL J.A.
	Astrophys. J., 211, 178-180 (1977)
	Photography at 9400 Angstroms of infrared and molecular line sources.
o	Table 1: <[CF77] Mon R2 N> (Nos 1-6), <[CF77] OMC 2 N> (Nos 1-2, 4). Plate 4, text: <[CF77] Mon R2 Star B>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CF77a]
[CF77a]	(Cohen+Frogel, 1977)
*****	Avoid the usage of [CF77a], prefer [CF77]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CF77b]
[CF77b]	(Canterna+Flower, 1977) (Not yet in Simbad)
Write:	<<[CF77b] N>>
N:	3
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	N=3 suspected globular clusters. In 1999AJ....118..862M, objects 1 and 2 are identified as background galaxies. See also [MGA99].
in source:	NAME Phe Dwarf Irregular
Ref:	=1977ApJ...212L..57C
by	CANTERNA R. , FLOWER P.J.
	Astrophys. J., 212, 57-58 (1977)
	A new dwarf irregular galaxy in the constellation Phoenix.
o	<NAME PHOENIX DWARF IRREGULAR>. Fig.1: <[CF77b] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CF95]
[CF95]	(Codella+Felli, 1995)
Write:	<<[CF95] NN>>
N:	60
Object:	H2O Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Ref:	=1995A&A...302..521C
by	CODELLA C. , FELLI M.
	Astron. Astrophys., 302, 521-527 (1995)
	H_{2}O masers without associated diffuse HII regions: an earlier evolutionary phase?
o	Table 1: WB = WB89, p. 524 : WB89 621 misprint for 261
o	Table 1: <[CF95] NN> (Nos 1-60)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CF97]
[CF97]	(Cellone+Forte, 1997)= ([CF97a])
Write:	<<[CF97] NO>> <<[CF97] NN>>
N:	1+30
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Fig. 1: one object is called by the authors 'NO' (North Object) Table 3: (Nos 1-30), N=30 knots or regions in NGC 1427A
in source:	NGC 1427A
Ref:	=1997AJ....113.1239C
by	CELLONE S.A. , FORTE J.C.
	Astron. J., 113, 1239-1249 (1997)
	The peculiar morphology of the irregular galaxy NGC 1427A.
o	Fig.1: <[CF97] NO> N=1. Table 3: <[CF97] NN> (Nos 1-30).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CF97a]
[CF97a]	(Cellone+Forte, 1997)
*****	Avoid the usage of [CF97a], prefer [CF97]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CF97b]
[CF97b]	(Craig+Fruscione, 1997)
Write:	<<[CF97b] EUVE JHHMM+DD.d N>>
N:	12
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 3, Fig.1: Possible optical identifications of N=6 EUVE sources
Ref:	=1997AJ....114.1356C
by	CRAIG N. , FRUSCIONE A.
	Astron. J., 114, 1356-1364 (1997)
	Optical identification of joint EUVE and ROSAT detections in the Southern Hemisphere: soft active galactic nuclei.
o	Table 3, Fig.1: <[CF97b] EUVE JHHMM-DD.d N> N=12
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CfA
CfA	(Center for Astrophysics)
*****	Avoid the usage of CfA, prefer GHCG
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CFB2003]
[CFB2003]	(Comeron+Fernandez+Baraffe+, 2003)
Write:	<<[CFB2003] Par-Lup3-N>> <<[CFB2003] Par-Lup3-1/cc1>>
N:	4+1
Object:	* (SIMBAD class: Star)
Note:	New members of the Lupus 3 dark cloud. In the format 'Par' stands for Paranal observatory, and '1/cc1' is a fifth star companion of star 1.
in source:	Lupus 3
Ref:	=2003A&A...406.1001C
by	COMERON F. , FERNANDEZ M., BARAFFE I., NEUHAEUSER R., KAAS A.A.
	Astron. Astrophys., 406, 1001-1017 (2003)
	New low-mass members of the Lupus 3 dark cloud: Further indications of pre-main-sequence evolution strongly affected by accretion.
o	Table 1: <[CFB2003] Par-Lup3-N> (Nos 1-4), <[CFB2003] Par-Lup3-1/cc1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFB2010]
[CFB2010]	(Castellano+Fontana+Boutsia+, 2010)
Write:	<<[CFB2010] GN NNNN>>
N:	9
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT Hawk-I NIR observations of galaxies in the GOODS-South field.
in source:	NAME GOODS South Field
Ref:	=2010A&A...511A..20C
by	CASTELLANO M. , FONTANA A., BOUTSIA K., GRAZIAN A., PENTERICCI L., BOUWENS R., DICKINSON M., GIAVALISCO M., SANTINI P., CRISTIANI S., FIORE F., GALLOZZI S., GIALLONGO E., MAIOLINO R., MANNUCCI F., MENCI N., MOORWOOD A., NONINO M., PARIS D., RENZINI A., ROSATI P., SALIMBENI S., TESTA V., VANZELLA E.
	Astron. Astrophys., 511A, 20-20 (2010)
	Evidence of a fast evolution of the UV luminosity function beyond redshift 6 from a deep HAWK-I survey of the GOODS-S field.
o	Table 1, Text: <[CFB2010] GN NNNN> N=7+2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFB2017]
[CFB2017]	(Cai+Fan+Bian+, 2017)
Write:	<<[CFB2017] BOSS1441>> <<[CFB2017] LAENN>>
N:	1+19
Object:	Overdensity + EmG (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	KPNO MOSAIC1.1 Mayall 4m telescope, LBT LBC and MODS observations of N=1 overdensity and N=19 Lyα emitters. Use of SDSS-III/BOSS data. See also [ZCA2021].
Ref:	=2017ApJ...839..131C
by	CAI Z. , FAN X., BIAN F., ZABLUDOFF A., YANG Y., PROCHASKA J.X., McGREER I., ZHENG Z.-Y., KASHIKAWA N., WANG R., FRYE B., GREEN R., JIANG L.
	Astrophys. J., 839, 131-131 (2017)
	Mapping the Most Massive Overdensities Through Hydrogen (MAMMOTH). II. Discovery of the extremely massive overdensity BOSS1441 at z = 2.32.
o	CDFSz28 and J1431+3239 were not identified.
o	<[CFB2017] BOSS1441> N=1. Fig. 7, Table 2: <[CFB2017] LAENN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFB83]
[CFB83]	(Ciardullo+Ford+Bartko+, 1983)
Write:	<<[CFB83] ACO NNNN-N>> <<[CFB83] 1451+22 Group NN-N>> <<[CFB83] 1615+43 Group NN-N>> <<[CFB83] 1451+22 Group NNA>> <<[CFB83] 1615+43 Group NN>>
N:	124+44
Object:	G + Group of G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 1: Galaxies in 2 superclusters 1451+22 (= MFJG 18) and 1615+43 (= MFJG 19) N=75+49 galaxies, in ACO or in groups in each SuperCl (see T.2) format 'ACO NNNN-N', '1451+22 Group NN-N' and '1615+43 Group NN-N' Table 2: Groups in each supercluster, format '1451+22 Group NNA' and '1615+43 Group NN'
in source:	MFJG 18
in source:	MFJG 19
Ref:	=1983ApJ...273...24C
by	CIARDULLO R. , FORD H., BARTKO F., HARMS R.
	Astrophys. J., 273, 24-35 (1983)
	Redshifts of groups and clusters in the rich superclusters 1451+22 and 1615+43.
o	supercl 1451+22 = MFJG 18, supercl 1615+43 = MFJG 19
o	Table 1: <[CFB83] ACO NNNN-N>, <[CFB83] 1451+22 Group NN-N>, <[CFB83] 1615+43 Group NN-N> N=124. Table 2: <[CFB83] 1451+22 Group NNA>, <[CFB83] 1615+43 Group NN> N=44
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFB97]
[CFB97]	(Cui+Feldkhun+Braun, 1997)
Write:	<<[CFB97] JHHMMSS+DDMMSS>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observation of NGC 4736 Detection of 2 sources: a nuclear source: '[CFB97] J125052+410710' an off-center source: '[CFB97] J125048+410735'
in source:	NGC 4736
Ref:	=1997ApJ...477..693C
by	CUI W. , FELDKHUN D., BRAUN R.
	Astrophys. J., 477, 693-699 (1997)
	Detection of compact nuclear X-ray emission in NGC 4736.
o	Table 2: <[CFB97] J125052+410710>, <[CFB97] J125048+410735>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CFBDS
CFBDS	(CFHT, Brown Dwarf Survey)
Write:	<<CFBDS JHHMMSS+DDMMSS>> <<CFBDS JHHMMSS.ss+DDMMSS.s>>
Object:	BD* (SIMBAD class: BrownD* = Brown Dwarf)
Note:	CFHT MegaCam survey to search for brown dwarfs. Only the first references are given here.
Ref:	=2008A&A...482..961D
by	DELORME P. , DELFOSSE X., ALBERT L., ARTIGAU E., FORVEILLE T., REYLE C., ALLARD F., HOMEIER D., ROBIN A.C., WILLOTT C.J., LIU M.C., DUPUY T.J.
	Astron. Astrophys., 482, 961-971 (2008)
	CFBDS J005910.90-011401.3: reaching the T-Y brown dwarf transition?
o	Text: <CFBDS JHHMMSS.ss+DDMMSS.s> N=2 = <CFBDS JHHMMSS+DDMMSS> N=2.
Ref:	=2008A&A...484..469D
by	DELORME P. , WILLOTT C.J., FORVEILLE T., DELFOSSE X., REYLE C., BERTIN E., ALBERT L., ARTIGAU E., ROBIN A.C., ALLARD F., DOYON R., HILL G.J.
	Astron. Astrophys., 484, 469-478 (2008)
	Finding ultracool brown dwarfs with MegaCam on CFHT: method and first results.
o	Text: <CFBDS JHHMMSS+DDMMSS> N=3 added. <CFBDS JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CFBDSIR
CFBDSIR	(Canada-France Brown Dwarf Survey-InfraRed)
Write:	<<CFBDSIR JHHMMSS+DDMMSSA>> <<CFBDSIR JHHMM+DDMMA>> (not recognised by Simbad, but found in literature) <<CFBDSIR HHMM>>
Object:	BD* (SIMBAD class: BrownD* = Brown Dwarf)
Note:	CFHT WIRCam and MegaCam and NTT SOFI observations of brown dwarfs. Only the first references citing CFBDSIR objects are given here.
Ref:	=2010A&A...518A..39D
by	DELORME P. , ALBERT L., FORVEILLE T., ARTIGAU E., DELFOSSE X., REYLE C., WILLOTT C.J., BERTIN E., WILKINS S.M., ALLARD F., ARZOUMANIAN D.
	Astron. Astrophys., 518A, 39-39 (2010)
	Extending the Canada-France Brown Dwarfs Survey to the near-infrared: first ultracool brown dwarfs from CFBDSIR.
o	Paragr. 3.3, Tables 3-5: <CFBDSIR JHHMMSS+DDMMSS> N=3.
Ref:	=2011ApJ...740..108L
by	LIU M.C. , DELORME P., DUPUY T.J., BOWLER B.P., ALBERT L., ARTIGAU E., REYLE C., FORVEILLE T., DELFOSSE X.
	Astrophys. J., 740, 108 (2011)
	CFBDSIR J1458+1013B: a very cold (>T10) brown dwarf in a binary system.
o	<CFBDSIR JHHMMSS+DDMMSSA> N=3.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CFC
CFC	(Coma Filament Catalogue)
*****	Avoid the usage of CFC, prefer ComaFC
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CFC2001]
[CFC2001]	(Clementini+Federici+Corsi+, 2001) (Not yet in Simbad)
Write:	<<[CFC2001] GNNN NNNNNN>>
N:	24
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Note:	HST observations of M31. Search for RR LYrae stars in 4 globular clusters in M31: SKHB 11, SKHB 64, SKHB 33, SKHB 322.
in source:	M 31:SKHB 11 = SKHB 11
in source:	M 31:SKHB 64 = SKHB 64
in source:	M 31:SKHB 33 = SKHB 33
in source:	M 31:SKHB 322 = SKHB 322
Ref:	=2001ApJ...559L.109C
by	CLEMENTINI G. , FEDERICI L., CORSI C., CACCIARI C., BELLAZZINI M., SMITH H.A.
	Astrophys. J., 559, 109-112 (2001)
	RR Lyrae variables in the globular clusters of M31: a first detection of likely candidates.
o	Fig.2: <[CFC2001] GNNN NNNNNN> N=24.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFC2014]
[CFC2014]	(Calanog+Fu+Cooray+, 2013)
Write:	<<[CFC2014] 1HERMES S250 J100030.6+024142 lens>>
N:	1
Object:	Grav. lens (SIMBAD class: GravLens = Gravitational Lens)
Note:	Keck and HST NIR observations of candidate lensing systems identified by the HERMES and H-ATLAS surveys.
Ref:	=2014ApJ...797..138C
by	CALANOG J.A. , FU H., COORAY A., WARDLOW J., MA B., AMBER S., BAKER A.J., BAES M., BOCK J., BOURNE N., BUSSMANN R.S., CASEY C.M., CHAPMAN S.C., CLEMENTS D.L., CONLEY A., DANNERBAUER H., DE ZOTTI G., DUNNE L., DYE S., EALES S., FARRAH D., FURLANETTO C., HARRIS A.I., IVISON R.J., KIM S., MADDOX S.J., MAGDIS G., MESSIAS H., MICHALOWSKI M.J., NEGRELLO M., NIGHTINGALE J., O'BRYAN J.M., OLIVER S.J., RIECHERS D., SCOTT D., SERJEANT S., SIMPSON J., SMITH M., TIMMONS N., THACKER C., VALIANTE E., VIEIRA J.D.
	Astrophys. J., 797, 138 (2014)
	Lens models of Herschel-selected galaxies from high-resolution near-IR observations.
o	Table 3: <[CFC2014] 1HERMES S250 J100030.6+024142 lens> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFC97]
[CFC97]	(Cote+Freeman+Carignan+, 1997)= (Cen) = (Sc) = (Scu)
Write:	<<[CFC97] Sc NN>> <<[CFC97] Cen NN>>
N:	39+13
Object:	Poss. Dwarf G (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
in source:	NAME SCL GROUP
in source:	Centaurus Cluster = ACO 3526
Ref:	=1997AJ....114.1313C
by	COTE S. , FREEMAN K.C., CARIGNAN C., QUINN P.J.
	Astron. J., 114, 1313-1329 (1997)
	Discovery of numerous dwarf galaxies in the two nearest groups of galaxies.
o	Table 3: <[CFC97] Sc NN> N=39 among (Nos 1-44). Table 4: <[CFC97] Cen NN> (Nos 2-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CFDF
CFDF	(Canada France Deep Fields survey)
Write:	<<CFDF HHh NNNNNN>>
N:	about 100000
Object:	G (SIMBAD class: Galaxy)
Note:	CFHT observations of 4 fields: 3h, 22h, 14h, 11h.
Ref:	=2001A&A...376..756M
by	McCRACKEN H.J. , LE FEVRE O., BRODWIN M., FOUCAUD S., LILLY S.J., CRAMPTON D., MELLIER Y.
	Astron. Astrophys., 376, 756-774 (2001)
	The Canada-France deep fields survey. I. 100000 galaxies, 1 °^{2}: A precise measurement of ω(θ) to I_{AB}~25.
o	Catalog: <CFDF HHh NNNNNN>.
Origin	of the Acronym: L (2003ApJ...582....6W,2004MNRAS.350..785W)
Details on Acronym: [CFG2001]
[CFG2001]	(Carter+Fabricant+Geller+, 2001)= ([CFG2001a])
Write:	<<[CFG2001] 15R HHMMSS.s+DDMMSS.s>>
N:	30
Object:	G (SIMBAD class: Galaxy)
Note:	N=30 most vigorous star-forming galaxies from the 15R-North galaxy redshift survey.
Ref:	=2001ApJ...559..606C
by	CARTER B.J. , FABRICANT D.G., GELLER M.J., KURTZ M.J., McLEAN B.
	Astrophys. J., 559, 606-619 (2001)
	Star formation in a complete spectroscopic survey of galaxies.
o	p. 609 : Cyg OB 2-9 is in fact Schulte 9.
o	Table 3: <[CFG2001] 15R HHMMSS.s+DDMMSS.s> N=30.
=E=	Catalogue in electronic form as J/ApJ/559/606
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFG2001a]
[CFG2001a]	(Carter+Fabricant+Geller+, 2001)
*****	Avoid the usage of [CFG2001a], prefer [CFG2001]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFG2001b]
[CFG2001b]	(Crawford+Fabian+Gandhi+, 2001)
Write:	<<[CFG2001b] AN>>
N:	2+4+2+4+2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra serendipitous X-ray sources in 5 Chandra fields: field P (ACO 426 field), I (IRAS 09104+4109 field), A (ACO 1795 field), B (ACO 1835 field), C (ACO 2199 field). See also [CGF2002] and [GCF2002].
Ref:	=2001MNRAS.324..427C
by	CRAWFORD C.S. , FABIAN A.C., GANDHI P., WILMAN R.J., JOHNSTONE R.M.
	Mon. Not. R. Astron. Soc., 324, 427-442 (2001)
	Infrared observations of serendipitous hard Chandra X-ray sources.
o	table 1: CXOU J091360.0+405548 = CXOU J091359.9+405548 in SIMBAD
o	Table 1: <[CFG2001b] AN> (Nos P1-P2, I1-I4, A1-A2, B1-B4, C1-C2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFG78]
[CFG78]	(Cheung+Frogel+Gezari+, 1978)
Write:	<<[CFG78] Peak R>>
N:	4
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	N=4 millimeter peaks in NGC 6334. See also MFSW
in source:	NGC 6334
Ref:	=1978ApJ...226L.149C
by	CHEUNG L. , FROGEL J.A., GEZARI D.Y., HAUSER M.G.
	Astrophys. J., 226, 149-152 (1978)
	1.0 millimeter continuum map of cool sources in the NGC 6334 complex.
o	Error in the journal table of contents (p.146 instead of p.149)
o	Table 1: <[CFG78] Peak R> (Nos I to IV)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFG91]
[CFG91]	(Cappi+Focardi+Gregorini+, 1991)
Write:	<<[CFG91] ACO NNNN N>>
N:	19
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=19 G in 10 rich ACO clusters G in ACO 2799, 2911, 3094, 3122, 3223 and 3341 have been completed in [GCF93].
in source:	ACO 2734
in source:	ACO 2799
in source:	ACO 2819
in source:	ACO 2911
in source:	ACO 3094
in source:	ACO 3122
in source:	ACO 3151
in source:	ACO 3223
in source:	ACO 3341
in source:	ACO 3809
Ref:	=1991A&AS...88..349C
by	CAPPI A. , FOCARDI P., GREGORINI L., VETTOLANI G.
	Astron. Astrophys., Suppl. Ser., 88, 349-353 (1991)
	Redshifts of southern rich clusters.
o	<Electronic table connected with 1993A&AS.101.259G>
o	Table 1: <[CFG91] ACO NNNN N> N=19
=E=	Catalogue in electronic form as J/A+AS/101/259
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFG97]
[CFG97]	(Chen+Fabian+Gendreau, 1997)= ([CFG97a])
Write:	<<[CFG97] NN>> <<[CFG97] SN>> <<[CFG97] QN>>
N:	92
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ASCA and ROSAT PSPC observations N=92 sources (Nos 1-92). The 3 brightest include one star 'S1' and 2 QSO 'Q1' and 'Q2'
Ref:	=1997MNRAS.285..449C
by	CHEN L.-W. , FABIAN A.C., GENDREAU K.C.
	Mon. Not. R. Astron. Soc., 285, 449-471 (1997)
	ASCA and ROSAT observations of the QSF3 field: the X-ray background in the 0.1-7 keV band.
o	T.2, col(6), Name = 'Shanks QXSF3:NN'
o	Table 2: <[CFG97] NN> (Nos 1-92), <[CFG97] S1> = <[CFG97] 11>, <[CFG97] Q1> = <[CFG97] 37>, <[CFG97] Q2> = <[CFG97] 41>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFG97a]
[CFG97a]	(Chen+Fabian+Gendreau, 1997)
*****	Avoid the usage of [CFG97a], prefer [CFG97]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFG97b]
[CFG97b]	(Claussen+Frail+Goss+, 1997)
Write:	<<[CFG97b] W28 NNA>> <<[CFG97b] W44 NNA>> <<[CFG97b] IC 443 NA>> <<[CFG97b] IC 443 NAN>> <<[CFG97b] W28 OH A>> <<[CFG97b] W44 OH A>>
N:	45+6+32+6+6+5
Object:	OH Maser (SIMBAD class: Maser)
Note:	In W 28: 'W28 NNA', N=41 (Nos 1-41) + 4 components (39A-39D), OH masers in W 28 'W28 OH A', N=6 (Nos A-F) regions of OH emission concentrations Map in 1st ref, Fig. 1 In W 44: 'W44 OH A', N=6 (Nos A-F) regions of OH emission concentrations 'W44 NNA', N=25 (Nos 1-25) OH masers + 7 components. The format NNA is sometimes found in the literature as 'ANNA', where the first digit 'A' stands for the condensation region. Map in Fig. 2 In IC 443: 'IC443 N', N=6 (Nos 1-6) OH masers in IC 443 'IC443 NA' and 'IC 443 NAN', features in masers.
in source:	W 28
in source:	W 44
in source:	IC 443
Ref:	=1997ApJ...489..143C
by	CLAUSSEN M.J. , FRAIL D.A., GOSS W.M., GAUME R.A.
	Astrophys. J., 489, 143-159 (1997)
	Polarization observations of 1720 MHz OH masers toward the three supernova remnants W28, W44, and IC 443.
o	p. 156: subclumps = [HDS86] IC443G1 and G2
o	Table 2: <[CFG97b] W28 NN> (Nos 1-41), <[CFG97b] W28 OH A> (Nos A-F). Table 3: <[CFG97b] W44 NN> (Nos 1-25), <[CFG97b] W44 OH A> (Nos A-F). Table 4: <[CFG97b] IC443 N> (Nos 1-6).
Ref:	=1999ApJ...522..349C
by	CLAUSSEN M.J. , GOSS W.M., FRAIL D.A., DESAI K.
	Astrophys. J., 522, 349-356 (1999)
	The sizes of 1720 MHz OH masers: VLBA and MERLIN observations of the supernova remnants W44 and W28.
o	Table 3: <[CFG97b] W28 NNA> (Nos 39A-39D).
Ref:	=2003ApJ...583..272H
by	HOFFMAN I.M. , GOSS W.M., BROGAN C.L., CLAUSSEN M.J., RICHARDS A.M.S.
	Astrophys. J., 583, 272-279 (2003)
	The sizes of OH (1720 MHz) supernova remnant masers: MERLIN and very long baseline array observations of IC 443.
o	Table 1: <[CFG97b] IC443 NA> (Nos 1A, 1B) added. Table 3: <[CFG97b] IC443 NAN> (Nos 1A1, 1A2, 1A3) added.
Ref:	=2005ApJ...627..803H
by	HOFFMAN I.M. , GOSS W.M., BROGAN C.L., CLAUSSEN M.J.
	Astrophys. J., 627, 803-812 (2005)
	The OH (1720 MHz) supernova remnant masers in W44: MERLIN and VLBA polarization observations.
o	Table 2: <[CFG97b] W44 NNA> (Nos 8A-8B, 11A-11C, 20A, 20B) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFG99]
[CFG99]	(Cotton+Feretti+Giovannini+, 1999) (Not yet in Simbad)
Write:	<<[CFG99] A>> <<[CFG99] AN>>
N:	6+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Study of features in the jet of NGC 315.
in source:	NGC 315
Ref:	=1999ApJ...519..108C
by	COTTON W.D. , FERETTI L., GIOVANNINI G., LARA L., VENTURI T.
	Astrophys. J., 519, 108-116 (1999)
	A parsec-scale accelerating radio jet in the giant radio galaxy NGC 315.
o	Fig.2, Table 4: <[CFG99] A> (Nos A-F), <[CFG99] AN> (No. A0).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: cfh12k
cfh12k	(Canada-France-Hawai 12K mosaic camera)
*****	Avoid the usage of cfh12k, prefer [SCH2004]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CFH85]
[CFH85]	(Ciardullo+Ford+Harms, 1985)
Write:	<<[CFH85] ACO NNNN-N>> <<[CFH85] HHMM+DDd-N>>
N:	109
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Galaxies in N=62 ACO clusters, format 'ACO NNNN-N', and in N=11 other clusters, format 'HHMM+DDd-N'.
Ref:	=1985ApJ...293...69C
by	CIARDULLO R. , FORD H., HARMS R.
	Astrophys. J., 293, 69-82 (1985)
	Cluster redshifts in five suspected superclusters.
o	<[CFH85] ACO NNNN-N> and <[CFH85] HHMM-DDd-N>, N=109
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CFHIZELS
CFHIZELS	(CF-HiZELS)
Write:	<<CFHIZELS -SM14-NNNNNN>>
N:	6315
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	CFHT WIRCam observations of N=6315 emission-line galaxies in a region of ∼10 square degrees in the SA22 field. Use of HiZELS, UKIDSS DXS DR10, and also VVDS and VIPERS data.
Ref:	=2015MNRAS.451.2303S
by	SOBRAL D. , MATTHEE J., BEST P.N., SMAIL I., KHOSTOVAN A.A., MILVANG-JENSEN B., KIM J.-W., STOTT J., CALHAU J., NAYYERI H., MOBASHER B.
	Mon. Not. R. Astron. Soc., 451, 2303-2323 (2015)
	CF-HiZELS, an ~ 10 °2 emission-line survey with spectroscopic follow-up: Hα, [OIII] + Hβ and [OII] luminosity functions at z = 0.8, 1.4 and 2.2.
o	Table A1: <CFHIZELS-SM14-NNNNNN> N=6315 among (Nos 4214-338460).
=E=	Catalogue in electronic form as J/MNRAS/451/2303
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CFHQS
CFHQS	(Canada-France High-z QSO Survey)
Write:	<<CFHQS JHHMMSS+DDMMSS>>
N:	4+6+9
Object:	QSO (SIMBAD class: QSO = Quasar)
Note:	Canada-France High-z Quasar Survey. CFHT MegaCam photometry. Gemini South GMOS and Hobby-Eberly telescope LRS spectroscopy.
Ref:	=2007AJ....134.2435W
by	WILLOTT C.J. , DELORME P., OMONT A., BERGERON J., DELFOSSE X., FORVEILLE T., ALBERT L., REYLE C., HILL G.J., GULLY-SANTIAGO M., VINTEN P., CRAMPTON D., HUTCHINGS J.B., SCHADE D., SIMARD L., SAWICKI M., BEELEN A., COX P.
	Astron. J., 134, 2435-2450 (2007)
	Four quasars above redshift 6 discovered by the Canada-France high-z quasar survey.
o	Table 1: <CFHQS JHHMMSS+DDMMSS> N=4.
Ref:	=2009AJ....137.3541W
by	WILLOTT C.J. , DELORME P., REYLE C., ALBERT L., BERGERON J., CRAMPTON D., DELFOSSE X., FORVEILLE T., HUTCHINGS J.B., McLURE R.J., OMONT A., SCHADE D.
	Astron. J., 137, 3541-3547 (2009)
	Six more quasars at redshift 6 discovered by the Canada-France high-z quasar survey.
o	Table 1: <CFHQS JHHMMSS+DDMMSS> N=6 added.
Ref:	=2010AJ....139..906W
by	WILLOTT C.J. , DELORME P., REYLE C., ALBERT L., BERGERON J., CRAMPTON D., DELFOSSE X., FORVEILLE T., HUTCHINGS J.B., McLURE R.J., OMONT A., SCHADE D.
	Astron. J., 139, 906-918 (2010)
	The Canada-France high-z quasar survey: nine new quasars and the luminosity function at redshift 6.
o	Table 1: <CFHQS JHHMMSS+DDMMSS> N=9 added.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CFHT
CFHT	(Canada-France-Hawaii Telescope)
*****	Avoid the usage of CFHT, prefer CFRS
Origin	of the Acronym: L (Veron)
Details on Acronym: CFHT
CFHT	(Canada-France-Hawaii Telescope`)
*****	Avoid the usage of CFHT, prefer [GDM2005]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CFHT
CFHT	(Canada-France-Hawaii Telescope)
*****	Avoid the usage of CFHT, prefer [MDM2001]
Origin	of the Acronym: L (2005ApJ...625..906M)
Details on Acronym: CFHT-BD-Tau
CFHT-BD-Tau	(CFHT, Brown Dwarf, Taurus)
Write:	<<CFHT-BD-Tau JHHMMSS.s+DDMMSS>>
N:	4+18
Object:	Brown Dwarf (SIMBAD class: BrownD* = Brown Dwarf)
Stat:	is completely incorporated in Simbad
Note:	CFHT search for Brown Dwarf candidates. See also[MDM2001].
in source:	NAME Taurus Region
Ref:	=2001ApJ...561L.195M
by	MARTIN E.L. , DOUGADOS C., MAGNIER E., MENARD F., MAGAZZU A., CUILLANDRE J.-C., DELFOSSE X.
	Astrophys. J., 561, 195-198 (2001)
	Four brown dwarfs in the Taurus star-forming region.
o	V410 Tau Anon 13 = [SS94] V410 Anon 13
o	Table 1: <[MDM2001] CFHT-BD-Tau N> (Nos 1-4) = <CFHT-BD-Tau JHHMMSS.s+DDMMSS> N=4.
Ref:	=2003IAUS..211...75M
by	MAGAZZU A. , DOUGADOS C., LICANDRO J., MARTIN E.L., MAGNIER E.A., MENARD F.
	211th Symposium of the IAU, held at the Outrigger Waikoloa Beach Hotel Waikoloa, Hawai, USA. 20-24 May 2002. Ed. by E.L. Martin. "Brown dwarfs"., 211, 75-78 (2003)
	Infrared spectra of brown dwarf candidates in Taurus.
o	Tables 1, 2: <CFHT-BD-Tau JHHMMSS.s+DDMMSS> N=18 added.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CFHTLS
CFHTLS	(Canada-France-Hawaii Telescope Legacy Survey)
Write:	<<CFHTLS NNNN NNNNNN>> <<CFHTLS NNNN_NNNNNN>> (not recognised by Simbad, but found in literature)
N:	35651677+2293851
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=35651677+2293851 sources respectively in the component "CFHTLS Deep" and "CFHTLS Wide" of the Canada-France-Hawaii Telescope Legacy Survey (CFHTLS). "CFHTLS Deep" comprises 4 independent 1 sq. deg. MegaCam pointings, and "CFHTLS Wide", 171 MegaCam pointings covering ∼155 sq. deg. in 4 contiguous patches. The unique object identifier NNNN NNNNNN is divided as follows: digit 1 indicates the survey (Deep=0, Wide=1), digit 2 indicates the patch index (1 for W1, etc.), digits 3 and 4 are the tile index, finally, digits 6-11 contain the object index in the survey/index/tile. For more information, visit the project website: http://www.cfht.hawaii.edu/Science/CFHTLS/
Ref:	=2012yCat.2317....0H
by	HUDELOT P. , CUILLANDRE J.C., WITHINGTON K., GORANOVA Y., McCRACKEN H., MAGNARD F., MELLIER Y., REGNAULT N., BETOULE M., AUSSEL H., KAVELAARS J.J., FERNIQUE P., BONNAREL F., OCHSENBEIN F., ILBERT O.
	yCat, 2317, 0 (2012)
	The final Canada-France-Hawaii Telescope Legacy Survey (CFHTLS) release.
o	<CFHTLS NNNN NNNNNN> N=35651677+2293851.
=E=	Catalogue in electronic form as <II/317/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CFHTLS
CFHTLS	(CFHT, Legacy Survey)
*****	Avoid the usage of CFHTLS, prefer [WDF2005]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CFHTLS-CL
CFHTLS-CL	(CFHT Legacy Survey, Cluster)
Write:	<<CFHTLS-CL JHHMMSS+DDMMSS>>
N:	169
Object:	Cl of G (SIMBAD class: ClG_Candidate = Cluster of Galaxies Candidate)
Note:	Cluster detection algorithm applied to the CFHTLS.
Ref:	=2007A&A...461...81O
by	OLSEN L.F. , BENOIST C., CAPPI A., MAUROGORDATO S., MAZURE A., SLEZAK E., ADAMI C., FERRARI C., MARTEL F.
	Astron. Astrophys., 461, 81-93 (2007)
	Galaxy clusters in the CFHTLS. First matched filter candidate catalogue of the Deep fields.
o	(Erratum) erratum vol. 478, p. 93 (2008)
o	Table 3: <CFHTLS-CL JHHMMSS+DDMMSS> N=169.
=E=	Catalogue in electronic form as J/A+A/461/81
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CFHTWIR-Oph
CFHTWIR-Oph	(CFHT WIRCam, rho Oph Cloud)
Write:	<<CFHTWIR-Oph NNN>>
N:	110
Object:	* (SIMBAD class: Star)
Note:	CFHT WIRCam observations of N=110 low-mass candidate members of the ρ Oph Cloud.
in source:	NAME rho Oph Cloud
Ref:	=2010A&A...515A..75A
by	ALVES DE OLIVEIRA C. , MORAUX E., BOUVIER J., BOUY H., MARMO C., ALBERT L.
	Astron. Astrophys., 515A, 75-75 (2010)
	The low-mass population of the ρ Ophiuchi molecular cloud.
o	Table 4: <CFHTWIR-Oph NNN> (Nos 1-110).
=E=	Catalogue in electronic form as J/A+A/515/A75
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CFJ2002]
[CFJ2002]	(Ciardullo+Feldmeier+Jacoby+, 2002)
Write:	<<[CFJ2002] NGC NNNN NN>>
N:	40+62+20+73+58+24
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	PNs in galaxies. See also Ford.
in source:	NGC 2403
in source:	NGC 3115
in source:	NGC 3351
in source:	NGC 3627
in source:	NGC 4258
in source:	NGC 5866
Ref:	=2002ApJ...577...31C
by	CIARDULLO R. , FELDMEIER J.J., JACOBY G.H., KUZIO DE NARAY R., LAYCHAK M.B., DURRELL P.R.
	Astrophys. J., 577, 31-50 (2002)
	Planetary nebulae as standard candles. XII. Connecting the population I and population II distance scales.
o	Table 2: <Ford M 31 NNN> (Nos 570-742) added. Table 3: <[CFJ2002] NGC 2403 NN> (Nos 1-40). Table 4: <[CFJ2002] NGC 3115 NN> (Nos 1-62). Table 5: <[CFJ2002] NGC 3351 NN> (Nos 1-20). Table 6: <[CFJ2002] NGC 3627 NN> (Nos 1-73). Table 7: <[CFJ2002] NGC 4258 NN> (Nos 1-58). Table 8: <[CFJ2002] NGC 5866 NN> (Nos 1-24).
=E=	Catalogue in electronic form as J/ApJ/577/31
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFJ83]
[CFJ83]	(Ciardullo+Ford+Jacoby, 1983)
Write:	<<[CFJ83] Nova N>>
N:	4
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Note:	Kitt Peak 0.9m telescope Hα observations of N=4 novae in M31.
in source:	M 31 = NGC 224
Ref:	=1983ApJ...272...92C
by	CIARDULLO R. , FORD H., JACOBY G.
	Astrophys. J., 272, 92-98 (1983)
	H-α observations of four novae in M 31.
o	Fig. 1, Table 2: <[CFJ83] Nova N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFK2002]
[CFK2002]	(Ciardullo+Feldmeier+Krelove+, 2002)
Write:	<<[CFK2002] NN>>
N:	21
Object:	Em. Obj. (SIMBAD class: EmObj = Emission Object)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-9) = PN-like emission-line objects. (Nos 10-21) = other blank-field emission-line objects.
Ref:	=2002ApJ...566..784C
by	CIARDULLO R. , FELDMEIER J.J., KRELOVE K., JACOBY G.H., GRONWALL C.
	Astrophys. J., 566, 784-793 (2002)
	A measurement of the contamination in [O III] λ5007 surveys of intracluster stars and the surface density of z=3.13 Lyα galaxies.
o	Tables 2, 4: <[CFK2002] NN> (Nos 1-21).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFK96]
[CFK96]	(Carkner+Feigelson+Koyama+, 1996)= (L1551X)
Write:	<<[CFK96] RX NN>> <<[CFK96] ASCA N>>
N:	38+7
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Table 1: ROSAT sources near the LDN 1551 cloud, (Nos RX 1 to RX 38) Table 2: ASCA sources near the LDN 1551 cloud, (Nos ASCA 1 to ASCA 7) Map in Fig. 2
in source:	LDN 1551
Ref:	=1996ApJ...464..286C
by	CARKNER L. , FEIGELSON E.D., KOYAMA K., MONTMERLE T., REID I.N.
	Astrophys. J., 464, 286-305 (1996)
	X-ray-emitting T Tauri stars in the L1551 cloud.
o	Table 1: <[CFK96] RX NN> (Nos 1-38). Table 2: <[CFK96] ASCA N> (Nos 1-7)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFM2016]
[CFM2016]	(Campbell+Friesen+Martin+, 2016)
Write:	<<[CFM2016] {D\|W}NN>>
N:	3
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	JCMT HCO+(3-2) and N2D+(3-2) molecular line observations of the Perseus molecular cloud.
in source:	NAME Perseus Molecular Cloud
Ref:	=2016ApJ...819..143C
by	CAMPBELL J.L. , FRIESEN R.K., MARTIN P.G., CASELLI P., KAUFFMANN J., PINEDA J.E.
	Astrophys. J., 819, 143 (2016)
	Contraction signatures toward dense cores in the Perseus molecular cloud.
o	Table 1: <[CFM2016] DNN> N=2 (Nos D26 and D38), <[CFM2016] W10>.
=E=	Catalogue in electronic form as J/ApJ/819/143
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFN87]
[CFN87]	(Ciardullo+Ford+Neill+, 1987)= (C) = CFNJS
Write:	<<[CFN87] NN>>
N:	40
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Stat:	is completely incorporated in Simbad
in source:	M 31 = NGC 224
Ref:	=1987ApJ...318..520C
by	CIARDULLO R. , FORD H.C., NEILL J.D., JACOBY G.H., SHAFTER A.W.
	Astrophys. J., 318, 520-530 (1987)
	The spatial distribution and population of novae in M 31.
o	table 2: field standards, not in Simbad
o	Table 3: <[CFN87] NN> (Nos 1-35).
Ref:	=1990ApJ...356..472C
by	CIARDULLO R. , SHAFTER A.W., FORD H.C., NEILL J.D., SHARA M.M., TOMANEY A.B.
	Astrophys. J., 356, 472-482 (1990)
	The H-α light curves of novae in M 31.
o	Table 3: <[CFN87] NN> (Nos 36-40) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFN94]
[CFN94]	(Codella+Felli+Natale+, 1994)
Write:	<<[CFN94] HHMMSS.s+DDMMSS>>
N:	17 among 68
Object:	H2O Maser (SIMBAD class: Maser)
Note:	Water maser sources found by the authors from Lockman HII regions [L89b]
Ref:	=1994A&A...291..261C
by	CODELLA C. , FELLI M., NATALE V., PALAGI F., PALLA F.
	Astron. Astrophys., 291, 261-270 (1994)
	The occurrence of H_{2}O masers in HII regions.
o	<[CFN94] HHMMSS.s+DDMMSS> N=17 among 68
=E=	Catalogue in electronic form as J/A+A/291/261
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CFNJS
CFNJS	(Ciardullo+Ford+Neill+Jacoby+Shafter)
====>	Equivalent to: [CFN87]
Origin	of the Acronym: L (2001ApJ...563..749S)
Details on Acronym: [CFP2008]
[CFP2008]	(Cenko+Fox+Penprase+, 2008) (Not yet in Simbad)
Write:	<<[CFP2008] {R\|B}N>>
N:	2+1
Object:	G (SIMBAD class: Galaxy)
Note:	Galaxies in the field of GRB 070125. The galaxy R1 is a possible host galaxy of the GRB.
Ref:	=2008ApJ...677..441C
by	CENKO S.B. , FOX D.B., PENPRASE B.E., CUCCHIARA A., PRICE P.A., BERGER E., KULKARNI S.R., HARRISON F.A., GAL-YAM A., OFEK E.O., RAU A., CHANDRA P., FRAIL D.A., KASLIWAL M.M., SCHMIDT B.P., SODERBERG A.M., CAMERON P.B., ROTH K.C.
	Astrophys. J., 677, 441-447 (2008)
	GRB 070125: the first long-duration γ-ray burst in a halo environment.
o	Fig.1: <[CFP2008] AN> (Nos B1, B2, R1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFP2010]
[CFP2010]	(Castellano+Fontana+Paris+, 2010)
Write:	<<[CFP2010] BDF NNNN>> <<[CFP2010] NTTDF NNNN>>
N:	21+7
Object:	G (SIMBAD class: Galaxy)
Note:	VLT Hawk-I NIR and FORS2 observations of z-drop candidates, in the BDF field (at 336.98-35.17) and New Technology Telescope Deep Field (NTTDF, at 181.36-7.72).
Ref:	=2010A&A...524A..28C
by	CASTELLANO M. , FONTANA A., PARIS D., GRAZIAN A., PENTERICCI L., BOUTSIA K., SANTINI P., TESTA V., DICKINSON M., GIAVALISCO M., BOUWENS R., CUBY J.-G., MANNUCCI F., CLEMENT B., CRISTIANI S., FIORE F., GALLOZZI S., GIALLONGO E., MAIOLINO R., MENCI N., MOORWOOD A., NONINO M., RENZINI A., ROSATI P., SALIMBENI S., VANZELLA E.
	Astron. Astrophys., 524A, 28-28 (2010)
	The bright end of the z ~ 7 UV luminosity function from a wide and deep HAWK-I survey.
o	Fig. 3, Table 3: <[CFP2010] BDF NNNN> (Nos 521, 3299, 5905), <[CFP2010] NTTDF NNNN> N=5 among (Nos 1479-6543).
Ref:	=2011ApJ...743..132P
by	PENTERICCI L. , FONTANA A., VANZELLA E., CASTELLANO M., GRAZIAN A., DIJKSTRA M., BOUTSIA K., CRISTIANI S., DICKINSON M., GIALLONGO E., GIAVALISCO M., MAIOLINO R., MOORWOOD A., PARIS D., SANTINI P.
	Astrophys. J., 743, 132 (2011)
	Spectroscopic confirmation of z ~ 7 Lyman break galaxies: probing the earliest galaxies and the epoch of reionization.
o	Table 1: <[CFP2010] NTTDF NNNN> (Nos 474, 2916) added, <[CFP2010] BDF NNNN> (Nos 2687, 2883, 5583, 5665) added. Table 2: <[PFV2011] NTT-NNNN> N=5 among (Nos 1806-7246), <[PFV2011] BDF-NNNN> N=8 among (Nos 2203-5889), <[PFV2011] GOODSS-NNNNN> N=4 among (Nos 48-15052).
Ref:	=2018ApJ...863L...3C
by	CASTELLANO M. , PENTERICCI L., VANZELLA E., MARCHI F., FONTANA A., DAYAL P., FERRARA A., HUTTER A., CARNIANI S., CRISTIANI S., DICKINSON M., GALLERANI S., GIALLONGO E., GIAVALISCO M., GRAZIAN A., MAIOLINO R., MERLIN E., PARIS D., PILO S., SANTINI P.
	Astrophys. J., 863L, 3-3 (2018)
	Spectroscopic investigation of a reionized galaxy overdensity at z = 7.
o	Table 1: <[CFP2010] BDF NNNN> N=14 among (Nos 187-2980) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFR2000]
[CFR2000]	(Carey+Feldman+Redman+, 2000)
Write:	<<[CFR2000] GLLL.l+B.b PN>> <<[CFR2000] GLLL.ll+B.bb PN>>
N:	20
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	SCUBA observations of MSX sources. N=20 (SMM) compact sources in 8 [CCE98b] clouds. Here G79.3+0.3 = [CCE98b] 79.27+0.38 + [CCE98b] 79.34+0.33 clouds. See also [CCE98b] and [PWC2006].
in source:	[CCE98b] 353.85+0.23
in source:	[CCE98b] 353.51-0.33
in source:	[CCE98b] 357.51+0.33
in source:	[CCE98b] 010.74-0.13
in source:	[CCE98b] 011.11-0.12
in source:	[CCE98b] 019.30+0.07
in source:	[CCE98b] 028.34+0.06
in source:	[CCE98b] 079.27+0.38
in source:	[CCE98b] 079.34+0.33
Ref:	=2000ApJ...543L.157C
by	CAREY S.J. , FELDMAN P.A., REDMAN R.O., EGAN M.P., MacLEOD J.M., PRICE S.D.
	Astrophys. J., 543, 157-161 (2000)
	Submillimeter observations of midcourse space experiment galactic infrared-dark clouds.
o	Text: <[CCE98b] LLL.ll+B.bb> N=4 added. Table 1, Fig.1: <[CFR2000] GLLL.ll+B.bb PN> N=11.
Ref:	=2003ApJ...586.1127R
by	REDMAN R.O. , FELDMAN P.A., WYROWSKI F., COTE S., CAREY S.J., EGAN M.P.
	Astrophys. J., 586, 1127-1135 (2003)
	Interactions between a bright young stellar object and the Midcourse Space Experiment infrared-dark cloud G79.3+0.3: an early stage of triggered formation.
o	Fig.1: <[CFR2000] G79.3+0.3 PN> (Nos P4-P5) added. Table 2: <[RFW2003] G79.3+0.3 P1 A> (Nos A-C).
Ref:	=2003ApJ...588L..37J
by	JOHNSTONE D. , FIEGE J.D., REDMAN R.O., FELDMAN P.A., CAREY S.J.
	Astrophys. J., 588, 37-40 (2003)
	The G11.11-0.12 infrared-dark cloud: anomalous dust and a nonmagnetic isothermal model.
o	Parag. 3 : L97 in Cygnus is a misprint for L977 (= LDN 977)
o	Fig.2: <[CFR2000] G11.11-0.12 PN> (Nos P2-P7) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CFRS
CFRS	(Canada-France Redshift Survey)
*****	Avoid the usage of CFRS, prefer [BAS98]
Origin	of the Acronym: L (1998ApJ...550...75L)
Details on Acronym: CFRS
CFRS	(Canada-France Redshift Survey)= (CFHT)
Write:	<<CFRS HH.NNNN>>
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Format 'HH.NNNN': 'HH' stands for the survey field, in hours of right ascension (always 2 digits: fields 00, 03, 10, 14, 22), 'NNNN' stands for the object number in the photometric catalog in the field (always 4 digits) Only 1st papers from CFRS are given.
Ref:	=1995MNRAS.276.1085H
by	HAMMER F. , CRAMPTON D., LILLY S.J., LE FEVRE O., KENET T.
	Mon. Not. R. Astron. Soc., 276, 1085-1100 (1995)
	The Canada-France redshift survey - VII. Optical counterparts of microjansky radio sources.
o	Table 1, col.(1): <15V NNa> (Nos 26a, 26b). Table 1, col.(3): <CFRS 14.NNNN> N=37.
Ref:	=1995ApJ...455...60L
by	LE FEVRE O. , CRAMPTON D., LILLY S.J., HAMMER F., TRESSE L.
	Astrophys. J., 455, 60-74 (1995)
	The Canada-France Redshift Survey. II. Spectroscopic program: data for the 0000-00 and 1000+25 fields.
o	Tables 2, 3: <CFRS 00.NNNN>, <CFRS 10.NNNN> N=303
Ref:	=1995ApJ...455...75L
by	LILLY S.J. , HAMMER F., LE FEVRE O., CRAMPTON D.
	Astrophys. J., 455, 75-87 (1995)
	The Canada-France Redshift Survey. III. "Single emission-line" objects, analysis of repeat observations, and spectroscopic identifications in the 1415+52 and 2215+00 fields.
o	Tables 2, 3: <CFRS 14.NNNN>, <CFRS 22.NNNN> N=413
Ref:	=1995ApJ...455...88H
by	HAMMER F. , CRAMPTON D., LE FEVRE O., LILLY S.J.
	Astrophys. J., 455, 88-95 (1995)
	The Canada-France Redshift Survey. IV. Spectroscopic selection effects and 0300+00 field spectroscopic data.
o	Table 1: <CFRS 03.NNNN> N=273
Ref:	=1996ApJ...464...79S
by	SCHADE D. , LILLY S.J., LE FEVRE O., HAMMER F., CRAMPTON D.
	Astrophys. J., 464, 79-91 (1996)
	Canada-france redshift survey. XI. Morphology of high-redshift field galaxies from high-resolution ground-based imaging.
o	Table 1: <CFRS 14.NNNN> N=143.
Ref:	=1997ApJ...481...49H
by	HAMMER F. , FLORES H., LILLY S.J., CRAMPTON D., LE FEVRE O., ROLA C., MALLEN-ORNELAS G., SCHADE D., TRESSE L.
	Astrophys. J., 481, 49-82 (1997)
	Canada-France Redshift Survey. XIV. Spectral properties of field galaxies up to z=1.
o	<CFRS HH.NNNN> N=410.
=E=	Catalogue in electronic form as J/ApJ/455/60
=E=	Catalogue in electronic form as J/ApJ/455/75
=E=	Catalogue in electronic form as J/ApJ/455/88
=E=	Catalogue in electronic form as J/ApJ/464/79
=E=	Catalogue in electronic form as J/ApJ/481/49
=E=	Catalogue in electronic form as VII/225
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CFRS
CFRS	(Canada-France Redshift Survey)
*****	Avoid the usage of CFRS, prefer CUDSS
Origin	of the Acronym: L (2006MNRAS.371..465S)
Details on Acronym: CFRS
CFRS	(Canada-France Redshift Survey)
*****	Avoid the usage of CFRS, prefer [ELG99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CFS
CFS	(Cape obs., Faint *)
====>	Equivalent to: CF
Details on Acronym: [CFS78]
[CFS78]	(Cruddace+Fritz+Shulman+, 1978)
Write:	<<[CFS78] GC X-N>>
N:	6
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Rocket obervations of the Galactic Center.
in source:	NAME Gal Center
Ref:	=1978ApJ...222L..95C
by	CRUDDACE R.G. , FRITZ G., SHULMAN S., FRIEDMAN H., McKEE J., JOHNSON M.
	Astrophys. J., 222, 95-98 (1978)
	High-resolution observations of X-ray sources at the Galactic Center.
o	Table 1: <[CFS78] GC X-N> (Nos X-1 to X-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFT2001]
[CFT2001]	(Chandar+Ford+Tsvetanov, 2001)
Write:	<<[CFT2001] NNN>>
N:	114
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of 114 compact star clusters in M 81.
in source:	M 81 = NGC 3031
Ref:	=2001AJ....122.1330C
by	CHANDAR R. , FORD H.C., TSVETANOV Z.
	Astron. J., 122, 1330-1341 (2001)
	Compact star clusters in M81. I. Data from Hubble space telescope wide field planetary camera 2 imaging.
o	Table 2: <[CFT2001] NNN> (Nos 1-114).
=E=	Catalogue in electronic form as J/AJ/122/1330
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFT2002]
[CFT2002]	(Corbel++Fender+Tzioumis+, 2002)
Write:	<<[CFT2002] Radio JHHMMSS.ss+DDMMSS.s>> <<[CFT2002] X-ray JHHMMSS.ss+DDMMSS.s>>
N:	1+3
Object:	(Rad) + (X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	The X-ray binary XTE J1550-564 is observed at X-ray and Radio wavelengths and at two epochs (March 11 and June 19 2002). A large jet is detected along the same axis, west and east of XTE J1550-564, the X-ray jet being coinciding with the Radio jet. Along the jet, an additional radio-source is first detected at 'J155055.97-562833.5', west of XTE J1550-564. 3 X-ray sources are detected along the axis of the jet: XTE J1550-564, a west X-ray source 'J155055.94-562833.5' coinciding with the radio-source, and a east X-ray source 'J155101.30-562836.9'. A fourth X-ray source is added 'J155053.05-562902.0' that does not lie along the jet axis.
Ref:	=2002IAUC.7795....2C
by	CORBEL S. , FENDER R., TZIOUMIS A.
	IAU Circ., 7795, 2-None (2002)
	XTE J1550-564.
o	<[CFT2002] Radio JHHMMSS.ss+DDMMSS.s> N=1.
Ref:	=2002Sci...298..196C
by	CORBEL S. , FENDER R.P., TZIOUMIS A.K., TOMSICK J.A., OROSZ J.A., MILLER J.M., WIJNANDS R., KAARET P.
	Science, 298, 196-199 (2002)
	Large-scale, decelerating, relativistic X-ray jets from the microquasar XTE J1550-564.
o	West X-ray source = [CFT2002] X-ray J155055.94-562833.5 = West radio source [CFT2002] Radio J155055.97-562833.5. East X-ray source = [CFT2002] X-ray J155101.30-562836.9.
o	<[CFT2002] X-ray JHHMMSS.ss+DDMMSS.s> N=2.
Ref:	=2003ApJ...582..945K
by	KAARET P. , CORBEL S., TOMSICK J.A., FENDER R., MILLER J.M., OROSZ J.A., TZIOUMIS A.K., WIJNANDS R.
	Astrophys. J., 582, 945-953 (2003)
	X-ray emission from the jets of XTE J1550-564.
o	<[CFT2002] X-ray JHHMMSS.ss+DDMMSS.s> N=1 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFT2022]
[CFT2022]	(Castellano+Fontana+Treu+, 2022)
Write:	<<[CFT2022] GHZN>>
N:	6
Object:	Poss. G (SIMBAD class: Galaxy_Candidate = Galaxy Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=6 galaxy candidates at z>9 in JWST NIRCam imaging data, as part of the GLASS-JWST Early Release Science Program on a parallel field of the Abell 2744 cluster. See also [MBP2022].
Ref:	=2022ApJ...938L..15C
by	CASTELLANO M. , FONTANA A., TREU T., SANTINI P., MERLIN E., LEETHOCHAWALIT N., TRENTI M., VANZELLA E., MESTRIC U., BONCHI A., BELFIORI D., NONINO M., PARIS D., POLENTA G., ROBERTS-BORSANI G., BOYETT K., BRADAC M., CALABRO A., GLAZEBROOK K., GRILLO C., MASCIA S., MASON C., MERCURIO A., MORISHITA T., NANAYAKKARA T., PENTERICCI L., ROSATI P., VULCANI B., WANG X., YANG L.
	Astrophys. J., 938L, 15 (2022)
	Early Results from GLASS-JWST. III. Galaxy Candidates at z ~9-15.
o	Figs 3-4, Table 1: <[CFT2022] GHZN> (Nos GHZ1-GHZ6).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [CFT97]
[CFT97]	(Cesaroni+Felli+Testi+, 1997) (Not yet in Simbad)
Write:	<<[CFT97] HHMMSS.ss+DDMMSS.s>>
N:	6+301
Object:	(Near IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Table 13: Knots detected with NOT telescope, N=6 Table 14: sources detected with TIRGO telescope, N=301
Ref:	=1997A&A...325..725C
by	CESARONI R. , FELLI M., TESTI L., WALMSLEY C.M., OLMI L.
	Astron. Astrophys., 325, 725-744 (1997)
	The disk-outflow system around the high-mass (proto)star IRAS 20126+4104.
o	Tables 13 et 14: sources IR not in SIMBAD
o	Tables 13, 14: <[CFT97] HHMMSS.ss+DDMMSS.s> N=6+301
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFV2007]
[CFV2007]	(Cocchia+Fiore+Vignali+, 2007)
Write:	<<[CFV2007] JHHMMSS.s+DDMMSS>>
N:	117
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	ESO 3.6m EFOSC2, VLT FORS1, and TNG DOLORES observations. Possible optical identifications of HELLAS2XMM sources.
Ref:	=2007A&A...466...31C
by	COCCHIA F. , FIORE F., VIGNALI C., MIGNOLI M., BRUSA M., COMASTRI A., FERUGLIO C., BALDI A., CARANGELO N., CILIEGI P., D'ELIA V., LA FRANCA F., MAIOLINO R., MATT G., MOLENDI S., PEROLA G.C., PUCCETTI S.
	Astron. Astrophys., 466, 31-40 (2007)
	The HELLAS2XMM survey. VIII. Optical identifications of the extended sample.
o	Table 1, cols(opt. ID): <[CFV2007] JHHMMSS.s+DDMMSS> N=117. Tables 1, 3, 4: <HELLAS2XMM JHHMMSS.s+DDMMSS> N=141.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CFW90]
[CFW90]	(Ciardullo+Ford+Williams, 1990)
Write:	<<[CFW90] Star NN>> <<[CFW90] Nova NN>>
N:	48+16
Object:	* + nova (SIMBAD class: Star)
Note:	Table II: format '2-NN', N=48 stars in the field of NGC 5128 Table III: format '3-NN', N=16 novae in NGC 5128
in source:	Cen A = NGC 5128
Ref:	=1990AJ.....99.1079C
by	CIARDULLO R. , FORD H.C., WILLIAMS R.E., TAMBLYN P., JACOBY G.H.
	Astron. J., 99, 1079-1087 (1990)
	The nova rate in the elliptical component of NGC 5128.
o	Table II: <[CFW90] Star NN> N=48. Table III: <[CFW90] Nova NN> N=16
=E=	Catalogue in electronic form as J/AJ/99/1079
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CFWM
CFWM	(Churchwell+Felli+Wood+Massi)
Note:	The authors' initials in second ref.
*****	Avoid the usage of CFWM, prefer GMR
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CFY2017]
[CFY2017]	(Cai+Fan+Yang+, 2017) (Not yet in Simbad)
Write:	<<[CFY2017] Source A>>
N:	2
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	KPNO MOSAIC1.1 and LBT LBC And MODS osbervations of N=2 sources in the field of the enormous Lyman α nebula MAMMOTH-1.
in source:	NAME MAMMOTH-1
Ref:	=2017ApJ...837...71C
by	CAI Z. , FAN X., YANG Y., BIAN F., PROCHASKA J.X., ZABLUDOFF A., McGREER I., ZHENG Z.-Y., GREEN R., CANTALUPO S., FRYE B., HAMDEN E., JIANG L., KASHIKAWA N., WANG R.
	Astrophys. J., 837, 71-71 (2017)
	Discovery of an enormous Lyα nebula in a massive galaxy overdensity at z = 2.3.
o	Source B is not in SIMBAD.
o	<NAME MAMMOTH-1> N=1. Figs 1-2: <[CFY2017] Source A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CG
CG	(Compact G)
*****	Avoid the usage of CG, prefer ACG
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CG
CG	(Case univ., G)
*****	Avoid the usage of CG, prefer CasG
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CG
CG	(Cometary Globule)
Write:	<<CG NNA>> <<CG NNW>> <<CG NNAN>>
N:	47
Object:	RFN (SIMBAD class: ComGlob = Cometary Globule / Pillar)
Stat:	is completely incorporated in Simbad
Note:	Most of the CG objects have tails pointing directly away from Centre 1 (08h15m - 44deg 30') or Centre 2 (07h46m - 46deg 30') In 1992JApA...13..217S, 1950 coordinates are remeasured for head and tail-end of most of CG Nos 1-38 (and subdivisions format NNA and NNAN).
Ref:	=1976MNRAS.175p..19H
by	HAWARDEN T.G. , BRAND P.W.J.L.
	Mon. Not. R. Astron. Soc., 175, part no 16, 19-22 (1976)
	Cometary globules and the structure of the Gum Nebula.
o	<CG NN> (Nos 1-12)
Ref:	=1976MNRAS.177p..69S
by	SANDQVIST A.
	Mon. Not. R. Astron. Soc., 177, part no 16, 69-71 (1976)
	Four more cometary globules in the Gum Nebula.
o	<CG NN> (Nos 13-16)
Ref:	=1983ApL....23..119Z
by	ZEALEY W.J. , NINKOV Z., RICE E., HARTLEY M., TRITTON S.B.
	Astrophys. Lett., 23, 119-131 (1983)
	Cometary globules in the Gum-Vela complex.
o	<CG NNA> (Nos 17-30, 32-36, and 31A, B, C)
Ref:	=1983A&A...117..183R
by	REIPURTH B.
	Astron. Astrophys., 117, 183-198 (1983)
	Star formation in Bok globules and low-mass clouds.
o	<CG NNA> (Nos 37, 38) and 31D, E. <GDC N> (Nos 1-7)
Ref:	=1992JApA...13..217S
by	SRIDHARAN T.K.
	J. Astrophys. Astron., 13, 217-239 (1992)
	Kinematics of the Cometary Globules in the Gum Nebula.
o	<CG NNA> and <CG NNAN> Nos 32A, B, Nos 22B1, 22B2
Ref:	=1995A&A...301..522L
by	LEFLOCH B. , LAZAREFF B.
	Astron. Astrophys., 301, 522-536 (1995)
	Cometary globules. II. Observational tests of radiation-driven implosion: the case of CG7S.
o	CG 7S is a new CG located South of CG 7.
o	<CG 7S> N=1.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CG
CG	(1st COS B, Gamma)
*****	Avoid the usage of CG, prefer 1CG
Details on Acronym: CG
CG	(2nd COS B, Gamma)
*****	Avoid the usage of CG, prefer 2CG
Details on Acronym: CG
CG	(Case univ., G)
Write:	<<NAME CG HHMM+DD>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Note:	CG 1432+53 = CasG 474, CG 1457+42 = CasG 598, CG 1517+39 = CasG 684.
Ref:	=1987ApJ...314L..33M
by	MOODY J.W. , KIRSHNER R.P., MacALPINE G.M., GREGORY S.A.
	Astrophys. J., 314, 33-37 (1987)
	Emission-line galaxies in the Bootes Void.
o	<NAME CG 1432+53>, <NAME CG 1457+42>, <NAME CG 1517+39>
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CG
CG	(Catalog General)
*****	Avoid the usage of CG, prefer PLX
Origin	of the Acronym: L (1965Obs....85..202K)
Details on Acronym: CG
CG	(Cesco+Gibson)
*****	Avoid the usage of CG, prefer Y-C
Details on Acronym: CG
CG	(Compact Group)
*****	Avoid the usage of CG, prefer [TC2003]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CG
CG	(Compact Group)
*****	Avoid the usage of CG, prefer [WTK99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CG
CG	(Cesco+Gibson)
*****	Avoid the usage of CG, prefer YC
Details on Acronym: CG-NGP
CG-NGP	(Corbally+Garrison, North Gal. Pole)
*****	Avoid the usage of CG-NGP, prefer CGG* NGP
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CG-SGP
CG-SGP	(Corbally+Garrison, South Gal. Pole)
*****	Avoid the usage of CG-SGP, prefer CGG* SGP
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 1CG
1CG	(1st Cos B, Gamma)= (CG)
Write:	<<1CG LLL+BB>>
N:	13
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Ref:	=1979Natur.277...17P
by	PINKAU K.
	Nature, 277, 17-21 (1979)
	Present status of γ-ray astronomy.
Details on Acronym: 2CG
2CG	(2nd Cos B, Gamma)= (CG)
Write:	<<2CG LLL+BB>>
N:	25
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	N=25, a 26th object is called '2CG 299-00' in 1988A&A...201..100R
Ref:	=1981ApJ...243L..69S
by	SWANENBURG B.N. , BENNETT K., BIGNAMI G.F., BUCCHERI R., CARAVEO P., HERMSEN W., KANBACH G., LICHTI G.G., MASNOU J.L., MAYER-HASSELWANDER H.A., PAUL J.A., SACCO B., SCARSI L., WILLS R.D.
	Astrophys. J., 243, 69-73 (1981)
	Second COS-B catalogue of high-energy γ-ray sources.
o	<2CG LLL+BB> N=25
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CG2001]
[CG2001]	(Cohen+Green, 2001)
Write:	<<[CG2001] GLLL.ll+B.bbW>>
N:	57
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio selected inventory of a region of the Gal plane centred on L=312deg, from MOST MGPS2 survey with mid-IR attributes from MSX.
Ref:	=2001MNRAS.325..531C
by	COHEN M. , GREEN A.J.
	Mon. Not. R. Astron. Soc., 325, 531-544 (2001)
	Extended Galactic emission at l=312°: a comparison of mid-infrared and radio continuum (843 MHz) images.
o	Table 1: <[CG2001] GLLL.ll+B.bbW> N=55.
Ref:	=2007MNRAS.374..979C
by	COHEN M. , GREEN A.J., MEADE M.R., BABLER B., INDEBETOUW R., WHITNEY B.A., WATSON C., WOLFIRE M., WOLFF M.J., MATHIS J.S., CHURCHWELL E.B.
	Mon. Not. R. Astron. Soc., 374, 979-998 (2007)
	Absolute diffuse calibration of IRAC through mid-infrared and radio study of HII regions.
o	In Chap. 10 : G313.45-0.13 is a misprint for G311.45-0.13
o	Table 1: <[CG2001] GLLL.ll+B.bb> (No. G311.70+0.31) added.
Ref:	=2009AJ....137.3449C
by	COHEN M.
	Astron. J., 137, 3449-3454 (2009)
	Absolute diffuse calibration of MIPS24 from a mid-infrared study of H II regions.
o	Table 1: <[CG2001] GLLL.ll+B.bb> (No. G311.82-0.29) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CG2007]
[CG2007]	(Ciardi+Gomez Martin, 2007)= (MIR)
Write:	<<[CG2007] MIR-a>>
N:	3
Object:	(Mid IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Gemini South T-ReCS MIR imaging observations of [CB88] 54.
in source:	[CB88] 54
Ref:	=2007ApJ...664..377C
by	CIARDI D.R. , GOMEZ MARTIN C.
	Astrophys. J., 664, 377-383 (2007)
	Star formation in the Bok globule CB 54.
o	Fig.1, Table 2: <[CG2007] MIR-a> (Nos a to c).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CG2010]
[CG2010]	(Connelley+Greene, 2010)
Write:	<<[CG2010] IRAS HHMMm+DDMM(W)>> <<[CG2010] IRAS 04181+2655(M)>> <<[CG2010] IRAS HHMMm+DDMM(WN)>> <<[CG2010] IRAS HHMMm+DDMM(N)>>
N:	50
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	NASA IRTF spectroscopic observations of Class I YSOs.
Ref:	=2010AJ....140.1214C
by	CONNELLEY M.S. , GREENE T.P.
	Astron. J., 140, 1214-1240 (2010)
	A near-infrared spectroscopic survey of class I protostars.
o	several IRAS names fixed in table2
o	Table 1: <[CG2010] IRAS HHMMm+DDMM(W)>, <[CG2010] IRAS HHMMm+DDMM(WN)>, <[CG2010] IRAS HHMMm+DDMM(N)> N=50.
=E=	Catalogue in electronic form as <J/AJ/140/1214/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CG88]
[CG88]	(Catelaz+Grasdalen, 1988)
Write:	<<[CG88] RNO-East>> <<[CG88] RNO-West>> <<[CG88] RNO>>
N:	2+1
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	NASA Infrared Telescope Facility observations. N=2 Red Nebular Objects (RNO) in NGC 2264.
in source:	NGC 2264
Ref:	=1988ApJ...335..150C
by	CASTELAZ M.W. , GRASDALEN G.
	Astrophys. J., 335, 150-156 (1988)
	The source of flux for a red nebulous object in NGC 2264.
o	Table 1: <[CG88] RNO-East>, <[CG88] RNO-West>. Text: <[CG88] RNO>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CG98]
[CG98]	(Castro-Tirado+Gorosabel, 1998)
Write:	<<[CG98] JHHMMSS.s+DDMMSS>>
N:	1
Object:	(Opt) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	N=1 variable object, candidate optical source of 1SAX J2329.6-2356. See also [GVV98].
Ref:	=1998GCN...173....1C
by	CASTRO-TIRADO A.J. , GOROSABEL J., DRORY N., KOENIG B., MOTTA V., GONZALEZ N., ACEITUNO J., GREINER J., FRONTERA F., PALAZZI E.
	GRB Coordinates Network, Circular Service, 173, 1-None (1998)
	GRB 981226 - infrared observations.
o	<[CG98] JHHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CG99]
[CG99]	(Conselice+Gallagher, 1999)= ([CG99a]) = (SA) = (SAWM)
Write:	<<[CG99] SANNNN-NNN>> <<[CG99] SAWMN-NN>>
N:	116+69+30+23+10
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Search for luminous fine-scale structures in 5 galaxy clusters. In the format 'SANNNN' stands for Structure in ACO NNNN, 'SAWMN' for Structure in AWM N.
in source:	ACO 1656 = Coma Cluster
in source:	ACO 426
in source:	ACO 2199
in source:	AWM 5
in source:	AWM 3
Ref:	=1999AJ....117...75C
by	CONSELICE C.J. , GALLAGHER III J.S.
	Astron. J., 117, 75-101 (1999)
	Tides, interactions, and fine-scale substructures in galaxy clusters.
o	Table 2: <[CG99] SA1656-NNN> (Nos 1-116). Table 3: <[CG99] SA426-NN> (Nos 1-69). Table 4: <[CG99] SA2199-NN> (Nos 1-30). Table 5: <[CG99] SAWM5-NN> (Nos 1-23). Table 6: <[CG99] SAWM3-NN> (Nos 1-10).
=E=	Catalogue in electronic form as J/AJ/117/75
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CG99a]
[CG99a]	(Conselice+Gallagher, 1999)
*****	Avoid the usage of [CG99a], prefer [CG99]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CG99b]
[CG99b]	(Churchwell+Goss, 1999)
Write:	<<[CG99b] NGC 604 A>> <<[CG99b] NGC 604 AN>> <<[CG99b] NGC 604 AAN>> <<[CG99b] Source R>>
N:	6+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	(Nos A-H) emission peaks, radio-components of NGC 604. Sub-regions 'AN' or 'AAN' are found. Sources I and II, N=2 radio-sources south of NGC 604.
in source:	NGC 604
Ref:	=1999ApJ...514..188C
by	CHURCHWELL E. , GOSS W.M.
	Astrophys. J., 514, 188-194 (1999)
	A high-resolution VLA and optical study of NGC 604.
o	Table 1: <[CG99b] NGC 604 A> (Nos A-F). Text: <[CG99b] Source R> (Nos I-II).
Ref:	=2004AJ....128.1196M
by	MAIZ-APELLANIZ J. , PEREZ E., MAS-HESSE J.M.
	Astron. J., 128, 1196-1218 (2004)
	NGC 604, the scaled OB association (SOBA) prototype. I. Spatial distribution of the different gas phases and attenuation by dust.
o	Figs 2, 3: Covity A to D are not in SIMBAD. Tables 3, 4: Subregions 'AN' et 'AAN' are not in SIMBAD.
o	Figs 2, 3: <[MPM2004] Cavity A> (Nos A-D). Tables 3, 4: <[CG99b] NGC 604 A> (Nos G-H) added, <[CG99b] NGC 604 AN> (Nos A1-A2, B1-B2, E1, F1-F2, G1-G4, H1-H2), <[CG99b] NGC 604 AAN> (Nos CD1-CD5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGA2008]
[CGA2008]	(Carrera+Gallart+Aparacio+, 2008)
Write:	<<[CGA2008] JHHMMSS.s+DDMMSS.s>>
N:	372
Object:	RGB* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 observations of Red Giant Branch (RGB) stars in the SMC. See also [CGH2008] in LMC.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2008AJ....136.1039C
by	CARRERA R. , GALLART C., APARICIO A., COSTA E., MENDEZ R.A., NOEL N.E.D.
	Astron. J., 136, 1039-1048 (2008)
	The chemical enrichment history of the Small Magellanic Cloud and its gradients.
o	Table 2: <[CGA2008] JHHMMSS.s+DDMMSS.s> N=372.
=E=	Catalogue in electronic form as <J/AJ/136/1039/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGA2011]
[CGA2011]	(Carrera+Gallart+Aparicio+, 2011)
Write:	<<[CGA2011] JHHMMSS.ss+DDMMSS.s>>
N:	249
Object:	RGB* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT FLAMES observations of Red Giant Branch (RGB) stars in the LMC.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2011AJ....142...61C
by	CARRERA R. , GALLART C., APARICIO A., HARDY E.
	Astron. J., 142, 61 (2011)
	Metallicities, age-metallicity relationships, and kinematics of red giant branch stars in the outer disk of the Large Magellanic Cloud.
o	Table 2: <[CGA2011] JHHMMSS.ss+DDMMSS.s> N=249.
=E=	Catalogue in electronic form as J/AJ/142/61
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGB2004a]
[CGB2004a]	(Cortese+Gavazzi+Boselli+, 2004)
Write:	<<[CGB2004a] JHHMMSS+DDMMSS>>
N:	6
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spectroscopic observations of six emission-line objects projected onto the Virgo Cluster at the 1.5m telescope at Loiano (Italy) and the 2.2m telescope at the Calar Alto Observatory (Spain).
Ref:	=2004A&A...416..119C
by	CORTESE L. , GAVAZZI G., BOSELLI A., IGLESIAS-PARAMO J.
	Astron. Astrophys., 416, 119-123 (2004)
	An extragalactic HII region in the Virgo cluster.
o	Table 3: <[CGB2004a] JHHMMSS+DDMMSS> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGB2004b]
[CGB2004b]	(Cortese+Gavazzi+Boselli+, 2004)
Write:	<<[CGB2004b] JHHMMSS+DDMMSS>>
N:	119
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=119 galaxies in ACO 1367. Most redshifts are from the WHT, the others from the Cassini 1.5m telescope at Loaino and the 2.1m telescope of the Guillermo Haro Observatory at Cananea. See also [IBG2003], [CGI2003].
in source:	ACO 1367
Ref:	=2004A&A...425..429C
by	CORTESE L. , GAVAZZI G., BOSELLI A., IGLESIAS-PARAMO J., CARRASCO L.
	Astron. Astrophys., 425, 429-441 (2004)
	Multiple merging in the Abell cluster 1367.
o	Table 7: <[CGB2004b] JHHMMSS+DDMMSS> N=119.
=E=	Catalogue in electronic form as J/A+A/425/429
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGB2005]
[CGB2005]	(Chatterjee+Goss+Brisken, 2005)
Write:	<<[CGB2005] JHHMMSS.sss+DDMMSS.ss>>
N:	15
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	NRAO VLA observations of the field of PSR J0737-3039.
Ref:	=2005ApJ...634L.101C
by	CHATTERJEE S. , GOSS W.M., BRISKEN W.F.
	Astrophys. J., 634, 101-104 (2005)
	Radio emission from the double-pulsar system J0737-3039 revisited.
o	Table 2: <[CGB2005] JHHMMSS.sss+DDMMSS.ss> N=15.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGB2013]
[CGB2013]	(Carretta+Gratton+Bragaglia+, 2013)
Write:	<<[CGB2013] NGC 7099 NNN>>
N:	8
Object:	* (SIMBAD class: Star)
Note:	ESO VLT UVES observations of N=8 stars in NGC 7099.
in source:	NGC 7099 = M 30
Ref:	=2013ApJ...769...40C
by	CARRETTA E. , GRATTON R.G., BRAGAGLIA A., D'ORAZI V., LUCATELLO S., SOLLIMA A., SNEDEN C.
	Astrophys. J., 769, 40 (2013)
	Potassium in globular cluster stars: comparing normal clusters to the peculiar cluster NGC 2419.
o	Table 1: <[CGB2013] NGC 7099 NNN> N=8 among (Nos 789-946).
=E=	Catalogue in electronic form as <J/ApJ/769/40/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGB2018]
[CGB2018]	(Cowie+Gonzalez-Lopez+Barger+, 2018)
Write:	<<[CGB2018] SMM JHHMMSS+DDMMSS>> <<[CGB2018] ALMA JHHMMSS+DDMMSS>> <<[CGB2018] SMMHHMMSS+DDMMSS>> (not recognised by Simbad, but found in literature) <<[CGB2018] ALMAHHMMSS+DDMMSS>>
N:	53+75
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	ALMA Band 7 (0.87mm) observations of N=75 sources and JCMT SCUBA-2 850µm observations of N=53 sources in the GOODS-South field. See also [CBH2017] for SCUBA-2 sources in the GOODS-North field.
in source:	NAME GOODS South Field
Ref:	=2018ApJ...865..106C
by	COWIE L.L. , GONZALEZ-LOPEZ J., BARGER A.J., BAUER F.E., HSU L.-Y., WANG W.-H.
	Astrophys. J., 865, 106-106 (2018)
	A submillimeter perspective on the GOODS fields (SUPER GOODS). III. A large sample of ALMA sources in the GOODS-S.
o	Table 2: <[CGB2018] SMM JHHMMSS+DDMMSS> N=53. Tables 4-5: <[CGB2018] ALMA JHHMMSS+DDMMSS> N=75.
=E=	Catalogue in electronic form as <J/ApJ/865/106/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGB2020]
[CGB2020]	(Carlsten+Greco+Beaton+, 2020)
Write:	<<[CGB2020] dwHHMM+DDMM>>
N:	139
Object:	Poss. Dwarf G (SIMBAD class: Galaxy_Candidate = Galaxy Candidate)
Note:	N=139 dwarf satellite candidates around 10 primary host galaxies in the Local Volume (LV, D<12Mpc) using archival CFHT/MegaCam imaging data. See also [CGP2020] and [CGG2021].
in source:	NGC 1023
in source:	NGC 1156
in source:	NGC 2903
in source:	NGC 4258
in source:	NGC 4565
in source:	NGC 4631
in source:	NGC 5023
in source:	NGC 5194 = M 51
in source:	NGC 4826 = M 64
in source:	Sombrero galaxy = NGC 4594 = M 104
Ref:	=2020ApJ...891..144C
by	CARLSTEN S.G. , GRECO J.P., BEATON R.L., GREENE J.E.
	Astrophys. J., 891, 144-144 (2020)
	Wide-field survey of dwarf satellite systems around 10 hosts in the Local Volume.
o	Tables 3-12: <[CGB2020] dwHHMM+DDMM> N=139.
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [CGB93]
[CGB93]	(Cristiani+Giallongo+Buson+, 1993)
Write:	<<[CGB93] HHMMSS.s+DDMMSS>>
N:	8
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Ref:	=1993A&A...268...86C
by	CRISTIANI S. , GIALLONGO E., BUSON L.M., GOUIFFES C., LA FRANCA F.
	Astron. Astrophys., 268, 86-92 (1993)
	Coordinated UV-optical observations of quasars : the evolution of the Lyman absorption.
o	Table 2: <[CGB93] HHMMSS.s+DDMMSS> N=8
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGC2004]
[CGC2004]	(Castro Ceron+Gorosabel+Castro-Tirado+, 2004)
Write:	<<[CGC2004] Star N>> <<[CGC2004] Object A>>
N:	8+2
Object:	* + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Optical and NIR follow up observations of GRB 001109. N=8 stars as photometric secondary standards in the field. NAME VLA J1830+5518 is separated in 2 objects A and B.
Ref:	=2004A&A...424..833C
by	CASTRO CERON J.M. , GOROSABEL J., CASTRO-TIRADO A.J., SOKOLOV V.V., AFANASIEV V.L., FATKHULLIN T.A., DODONOV S.N., KOMAROVA V.N., CHEREPASHCHUK A.M., POSTNOV K.A., LISENFELD U., GREINER J., KLOSE S., HJORTH J., FYNBO J.P.U., PEDERSEN H., ROL E., FLIRI J., FELDT M., FEULNER G., ANDERSEN M.I., JENSEN B.L., PEREZ RAMIREZ M.D., VRBA F.J., HENDEN A.A., ISRAELIAN G., TANVIR N.R.
	Astron. Astrophys., 424, 833-839 (2004)
	On the constraining observations of the dark GRB 001109 and the properties of a z = 0.398 radio selected starburst galaxy contained in its error box.
o	VLA J1830+5518 = NAME VLA J1830+5518 in SIMBAD.
o	Table 2: <[CGC2004] Star N> (Nos 1-8). Fig.4: <[CGC2004] Object A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGC2005]
[CGC2005]	(Chu+Gruendl+Chen+, 2005)
Write:	<<[CGC2005] YSO-N>>
N:	3
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Note:	Spitzer Space Telescope and Hubble Space Telescope observations of the supperbubble LHA 120-N 51.
in source:	Magellanic Clouds:LMC:LHA 120-N 51D = LHA 120-N 51D
Ref:	=2005ApJ...634L.189C
by	CHU Y.-H. , GRUENDL R.A., CHEN C.-H.R., WHITNEY B.A., GORDON K.D., LOONEY L.W., CLAYTON G.C., DICKEL J.R., DUNNE B.C., POINTS S.D., SMITH R.C., WILLIAMS R.M.
	Astrophys. J., 634, 189-192 (2005)
	Protostars, dust globules, and a Herbig-Haro object in the LMC superbubble N51D.
o	Object 4 = [O96] L54S-81
o	Figs, text: <[CGC2005] YSO-N> (Nos YSO-1 to YSO-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGC2008]
[CGC2008]	(Caulet+Gruendl+Chu+, 2008)
Write:	<<[CGC2008] JHHMMSS.ss+DDMMSS.s>> <<[CGC2008] N63 NN>> <<[CGC2008] N180 NN>> <<[CGC2008] N63 NNC>> <<[CGC2008] N180 NNC>>
N:	18+29+38
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Note:	Spitzer IR observations to find YSOs in the 2 LMC HII regions LHA 120-N 63 and LHA 120-N 180. Use of archival 2MASS data.
in source:	Magellanic Clouds:LMC:LHA 120-N 63 = LHA 120-N 63
in source:	Magellanic Clouds:LMC:LHA 120-N 180 = LHA 120-N 180
Ref:	=2008ApJ...678..200C
by	CAULET A. , GRUENDL R.A., CHU Y.-H.
	Astrophys. J., 678, 200-218 (2008)
	Young stellar objects in the Large Magellanic Cloud: N63 and N180 H II regions.
o	Table 3: <[CGC2008] JHHMMSS.ss+DDMMSS.s> N=18. Table 5: <[CGC2008] N63 NN>, <[CGC2008] N63 NNC>, N=29 among (Nos 8-50). Table 6: <[CGC2008] N180 NN>, <[CGC2008] N180 NNC>, N=38 among (Nos 9-45).
=E=	Catalogue in electronic form as J/ApJ/678/200
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGC2010]
[CGC2010]	(Chung+Gonzalez+Clowe+, 2010)
Write:	<<[CGC2010] JHHMMSS.ss+DDMMSS.ss>>
N:	12
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spitzer MIPS and IRAC, ESO 2.2m WFI and Magellan IMACS observations of N=12 spectroscopically confirmed members of the Bullet Cluster.
in source:	NAME BULLET CLUSTER = ClG 0657-56
Ref:	=2010ApJ...725.1536C
by	CHUNG S.M. , GONZALEZ A.H., CLOWE D., MARKEVITCH M., ZARITSKY D.
	Astrophys. J., 725, 1536-1549 (2010)
	Star formation in the Bullet cluster. I. The infrared luminosity function and star formation rate.
o	Table 2: <[CGC2010] JHHMMSS.ss+DDMMSS.ss> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGC2014]
[CGC2014]	(Carraro+Giorgi+Costa+, 2014)
Write:	<<[CGC2014] NNNN>>
N:	8197
Object:	* (SIMBAD class: Star)
Note:	Cerro Tololo 0.9m and 1m telescope photometric observations of N=8197 stars in the field of the open cluster NGC 4337.
in source:	NGC 4337
Ref:	=2014MNRAS.441L..36C
by	CARRARO G. , GIORGI E.E., COSTA E., VAZQUEZ R.A.
	Mon. Not. R. Astron. Soc., 441L, 36-40 (2014)
	NGC 4337: an overlooked old cluster in the inner disc of the Milky Way.
o	Table 2: <[CGC2014] NNNN> (Nos 1-8197).
=E=	Catalogue in electronic form as J/MNRAS/441/L36
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGC2015]
[CGC2015]	(Cusano+Garofalo+Clementini +, 2015)
Write:	<<[CGC2015] VNN>>
N:	50
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Large Binocular Telescope photometry of Andromeda XXI for identification of N=50 RR Lyrae and anomalous Cepheids stars. See also [CCG2013b] and [CGC2016].
in source:	And XXI
Ref:	=2015ApJ...806..200C
by	CUSANO F. , GAROFALO A., CLEMENTINI G., CIGNONI M., FEDERICI L., MARCONI M., MUSELLA I., RIPEPI V., SPEZIALI R., SANI E., MERIGHI R.
	Astrophys. J., 806, 200 (2015)
	Variable stars and stellar populations in Andromeda XXI. II. Another merged galaxy satellite of M31?
o	Table 2: <[CGC2015] VNN> (Nos V1-V50)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGC2016]
[CGC2016]	(Cusano+Garofalo+Clementini+, 2016)
Write:	<<[CGC2016] VNN>>
N:	62
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	Large Binocular Telescope photometry of Andromeda XXV for identification of N=62 variable stars. See also [CCG2013b] and [CGC2015].
in source:	And XXV
Ref:	=2016ApJ...829...26C
by	CUSANO F. , GAROFALO A., CLEMENTINI G., CIGNONI M., FEDERICI L., MARCONI M., RIPEPI V., MUSELLA I., TESTA V., CARINI R., FACCINI M.
	Astrophys. J., 829, 26-26 (2016)
	Variable stars and stellar populations in Andromeda XXV. III. A central cluster or the galaxy nucleus?
o	<NAME Gep I>. Table 2: <[CGC2016] VNN> N=62 among (Nos V1-V63).
=E=	Catalogue in electronic form as J/ApJ/829/26
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGC2017]
[CGC2017]	(Cusano+Garofalo+Clementini+, 2017)
Write:	<<[CGC2017] VNN>>
N:	90
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Note:	Large Binocular Telescope photometry of Andromeda XXVII for identification of N=90 variable stars. See also [CCG2013b], [CGC2015] and [CGC2016].
in source:	And XXVII
Ref:	=2017ApJ...851....9C
by	CUSANO F. , GAROFALO A., CLEMENTINI G., CIGNONI M., MURAVEVA T., TESSICINI G., TESTA V., PARIS D., FEDERICI L., MARCONI M., RIPEPI V., MUSELLA I.
	Astrophys. J., 851, 9-9 (2017)
	Variable stars and stellar populations in Andromeda XXVII. IV. An off-centered, disrupted galaxy.
o	Table 2: <[CGC2017] VNN> (Nos V1-V90).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGC77]
[CGC77]	(Clark+Giguere+Crutcher, 1977)= (DL)
Write:	<<[CGC77] DL N>>
N:	2
Object:	Dust Lane (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=2 dust condensations (Dust Lanes) in Taurus complex.
in source:	NAME Taurus Complex
Ref:	=1977ApJ...215..511C
by	CLARK F.O. , GIGUERE P.T., CRUTCHER R.M.
	Astrophys. J., 215, 511-516 (1977)
	Radio observations of fragmentation and localized multiple velocity components in a group of dust clouds in Taurus.
o	Fig.1: <[CGC77] DL N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGC93]
[CGC93]	(Chandler+Gear+Chini, 1993)= (FIR)
Write:	<<[CGC93] FIR NNa>>
N:	12+1
Object:	(Far IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	FIR sources observed were already present in 1986ApJ...300..737H but without an FIR designation.
in source:	DR 21 (OH)
Ref:	=1993MNRAS.260..337C
by	CHANDLER C.J. , GEAR W.K., CHINI R.
	Mon. Not. R. Astron. Soc., 260, 337-342 (1993)
	Dust emission associated with DR 21 (OH).
o	p. 340: CO-7 and NH3-3 are respectively: [WM90] W 75 CO 7 AND [WM90] W 75 NH3 3
o	Table 1: <[RSK89] DR 21(OH) N1>, <[RSK89] DR 21(OH) N2>. Table 1: <[CGC93] FIR N> (Nos 1-3)
Ref:	=2007MNRAS.374...29D
by	DAVIS C.J. , KUMAR M.S.N., SANDELL G., FROEBRICH D., SMITH M.D., CURRIE M.J.
	Mon. Not. R. Astron. Soc., 374, 29-53 (2007)
	WFCAM, Spitzer/IRAC and SCUBA observations of the massive star-forming region DR21/W75 - I. The collimated molecular jets.
o	Table 1 col(1): <[DKS2007] NN> (Nos 1-37). Fig.2, Table 1, col(9): <[DKS2007] DR21-IRSNN> (Nos 1-10). Fig.3, Table 1, col(9): <[DKS2007] W75N-IRSNN> (Nos 1-14). Fig.6, Table 1, col(9): <[DKS2007] L906E-IRSN> (Nos 1-6). Table 2: <[DKS2007] DR21WW>, <[DKS2007] DR21WN>, N=5, <[DKS2007] DR21(OH)WW> N=5, <[DKS2007] W75NWN>, N=8. Table 3: <[DKS2007] A NN-N> N=81. Table 4, col(2): <[DKS2007] a> (Nos a-n, i missing). Table 2: <[CGC93] FIR NNa> (Nos 4-12, 5b) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGC95]
[CGC95]	(Cool+Grindlay+Cohn+, 1995)
Write:	<<[CGC95] N>> <<[CGC95] NN>>
N:	15
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Note:	Table 2. HST Planetary Camera, FOC observations. See also [CGC98]
in source:	NGC 6397
Ref:	=1995ApJ...439..695C
by	COOL A.M. , GRINDLAY J.E., COHN H.N., LUGGER P.M., SLAVIN S.D.
	Astrophys. J., 439, 695-704 (1995)
	Discovery of candidate cataclysmic variables in the post-core-collapse globular cluster NGC 6397.
o	Table 2: <[CGC95] N> N=9
Ref:	=2010ApJ...722...20C
by	COHN H.N. , LUGGER P.M., COUCH S.M., ANDERSON J., COOL A.M., VAN DEN BERG M., BOGDANOV S., HEINKE C.O., GRINDLAY J.E.
	Astrophys. J., 722, 20-32 (2010)
	Identification of faint Chandra X-ray sources in the core-collapsed globular cluster NGC 6397: evidence for a bimodal cataclysmic variable population.
o	(Erratum) erratum vol. 930, art. 96 (2022)
o	Table 1: <[CGC95] NN> (Nos 10-15) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGC97]
[CGC97]	(Crampton+Gussie+Cowley+, 1997)
Write:	<<[CGC97] JHHMM.m+DDMM>>
N:	154
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Note:	Table 3 N=154 QSO candidates behind 9 nearby galaxies. Internal ID symbol used in col(2) is not used in SIMBAD. Maps in figs 6-15.
Note:	See also [CR82], [CP83], [CSC85], [CC87], [CCH87], [CCS88], [CCH90], [CCH91], [CCH92]
Ref:	=1997AJ....114.2353C
by	CRAMPTON D. , GUSSIE G., COWLEY A.P., SCHMIDTKE P.C.
	Astron. J., 114, 2353-2365 (1997)
	Probes for nearby galaxies.
o	in ref list: Garilli 1992AJ.104.1290
o	Table 3: <[CGC97] JHHMM.M+DDMM> N=154
=E=	Catalogue in electronic form as J/AJ/114/2353
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGC98]
[CGC98]	(Cool+Grindlay+Cohn+, 1998)= (CV) = (NF)
Write:	<<[CGC98] CV N>> <<[CGC98] NF N>> <<[CGC98] REF N>>
N:	5+3+3
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of NGC 6397. N=5 Cataclysmic Variables (Nos CV 1 to CV 5), CV5 added in 1999 Metchev Thesis. N=3 Non-Flickerers (Nos NF 1 to NF 3). N=3 reference stars (Nos REF 1 to REF 3). See also [CGC95]
in source:	NGC 6397
Ref:	=1998ApJ...508L..75C
by	COOL A.M. , GRINDLAY J.E., COHN H.N., LUGGER P.M., BAILYN C.D.
	Astrophys. J., 508, 75-79 (1998)
	Cataclysmic variables and a new class of faint ultraviolet stars in the globular cluster NGC 6397.
o	Table 1: <[CGC98] AA N> (Nos CV 1 to 4, Nos NF 1 to 3). Text: <[CGC98] AAA N> (Nos REF 1 to 3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CGCG
CGCG	(Catalog of G and Clusters of G)
Note:	Z for galaxies, ZwCl for ClG
**	catalog: use Z
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CGCG
CGCG	(Catalog of G and Clusters of G)
Note:	ZwCl for ClG, Z for galaxies
**	catalog: use ZwCl
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CGCS
CGCS	(Cool Gal. Carbon *)= (CGCS3) = (CS)
Write:	<<CGCS NNNN>>
N:	6891
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Note:	Last update in 2001. Same numbering is used but for new entries, but with running numbers beginning with No. 6001. See also [M2003b] temporary designations.
Ref:	=1989PW&SO...3...53S
by	STEPHENSON C.B.
	Publ. Warner & Swasey Obs., 3, 53-214 (1989)
	A general catalog of cool galactic carbon stars, second edition.
o	p.144: CGCS 3824 = C* 2439 (not 2429, misprint). p.159: CGCS 4711 = C* 2871 (not 871, misprint)
o	<CGCS NNNN> (Nos 1-5987)
Ref:	=2001BaltA..10....1A
by	ALKSNIS A. , BALKLAVS A., DZERVITIS U., EGLITIS I., PAUPERS O., PUNDURE I.
	Baltic Astronomy, 10, 1-318 (2001)
	General catalog of galactic carbon stars by C.B. Stephenson. Third edition.
o	(Erratum) Erratum vol.10 p.461 (2001)
o	The correct table is available in BaltA, vol.10, pp.461-477 (2001).
o	Catalogue: <CGCS NNNN> N=6891, with (Nos 6001-6924) added.
=E=	Catalogue in electronic form as III/156
=E=	Catalogue in electronic form as III/227
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CGCS3
CGCS3	(Cool Gal. Carbon *, 3rd edition)
*****	Avoid the usage of CGCS3, prefer CGCS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CGD2000]
[CGD2000]	(Cecil+Greenhill+DePree+, 2000)
Write:	<<[CGD2000] W Hot Spot>> <<[CGD2000] W Shock>>
N:	2+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=2 radio hot spots in NGC 4258 and N=2 emission line nebulae (shock front) enveloping the hot spots.
in source:	NGC 4258
Ref:	=2000ApJ...536..675C
by	CECIL G. , GREENHILL L.J., DEPREE C.G., NAGAR N., WILSON A.S., DOPITA M.A., PEREZ-FOURNON I., ARGON A.L., MORAN J.M.
	Astrophys. J., 536, 675-696 (2000)
	The active jet in NGC 4258 and its associated shocks.
o	Figures, text: outflows, jets and arms are not considered as individuals objects in SIMBAD.
o	Fig.3, Table 3: <[CGD2000] W Hot Spot> (Nos N, S), <[CGD2000] W Shock> (Nos N, S).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CGF
CGF	(Catalog of Galaxies in Fornax)
Write:	<<CGF FF-NNN>>
N:	873
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Catalog of galaxies in 11 fields 'FF' (1 to 11) in the Fornax Cluster, ordered with increasing distance to the center of the Fornax cluster. In each field, the galaxies numbering is ordered by decreasing magnitude.
in source:	NAME Fornax Cluster
Ref:	=1999A&AS..134...59H
by	HILKER M. , KISSLER-PATIG M., RICHTLER T., INFANTE L., QUINTANA H.
	Astron. Astrophys., Suppl. Ser., 134, 59-73 (1999)
	The central region of the Fornax cluster. I. A catalog and photometric properties of galaxies in selected CCD fields.
o	Table 4: cross-id col(3): NG NNN, col(4): FCC NNN or FCC BNNNN, col(5): FLSBG.
o	Appendix a, b: <CGF FF-NNN> N=873.
=E=	Catalogue in electronic form as J/A+AS/134/59
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CGF2002]
[CGF2002]	(Crawford+Gandhi+Fabian+, 2002)
Write:	<<[CGF2002] ANN>>
N:	31
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of 31 serendipitous X-ray sources in the field of ACO 2390. See also [CFG2001b] and [GCF2002].
Ref:	=2002MNRAS.333..809C
by	CRAWFORD C.S. , GANDHI P., FABIAN A.C., WILMAN R.J., JOHNSTONE R.M., BARGER A.J., COWIE L.L.
	Mon. Not. R. Astron. Soc., 333, 809-824 (2002)
	Multiwavelength observations of serendipitous Chandra X-ray sources in the field of A2390.
o	Table 1: <[CGF2002] ANN> (Nos A1-A31).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGF99]
[CGF99]	(Claussen+Goss+Frail+, 1999)
Write:	<<[CGF99] W44 Maser>>
N:	1
Object:	Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	W44 Maser previously discovered by Seta+ 1997, in 'Twenty-five years of millimeter-wave spectroscopy'. It marks the position of a late type giant or supergiant star, not related to the SNR. No detection towards IC 443, W28.
in source:	W 44
Ref:	=1999AJ....117.1387C
by	CLAUSSEN M.J. , GOSS W.M., FRAIL D.A., SETA M.
	Astron. J., 117, 1387-1391 (1999)
	No water masers associated with supernova remnants.
o	[CGF99] W44 Maser has been previously discovered by Sη+ 1997 (publication not in SIMBAD).
o	Table 6: <[CGF99] W44 Maser> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: *CGG NGP**
*CGG NGP**	(Corbally+Garrison, G *, North Gal. Pole)= (CG-NGP)
Write:	<<*CGG NGP** NNN>>
N:	192
Object:	Dw. * (SIMBAD class: Star)
Note:	The authors use the designation 'CG-NGP', which can't be used in SIMBAD Plates See also CGG* SGP
in source:	NAME NGP
Ref:	=1988AJ.....95..745C
by	CORBALLY C.J. , GARRISON R.F.
	Astron. J., 95, 745-749 (1988)
	A search for early-G dwarf stars the North Galactic Pole.
o	Table II: <CG-NGP NNN> use <CGG* NGP NNN>, (Nos 1-192)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: *CGG SGP**
*CGG SGP**	(Corbally+Garrison, G *, South Gal. Pole)= (CG-SGP)
Write:	<<*CGG SGP** NNN>>
N:	214
Object:	Dw. * (SIMBAD class: Star)
Note:	The authors use the designation 'CG-SGP', which can't be used in SIMBAD Plates See also CGG* NGP
in source:	NAME SGP
Ref:	=1988AJ.....95..739C
by	CORBALLY C.J. , GARRISON R.F.
	Astron. J., 95, 739-744 (1988)
	A search for early-G dwarf stars towards the South Galactic Pole.
o	Table III: <CG-SGP NNN> use <CGG* SGP NNN> (Nos 1-214)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGG2010]
[CGG2010]	(Cassata+Giavalisco+Guo+, 2010)
Write:	<<[CGG2010] NNNNN>>
N:	6
Object:	G (SIMBAD class: Galaxy)
Note:	HST WFC3 observations of N=6 passive and massive galaxies, selected from the GOODS survey in the Hubble Ultra Deep Field.
in source:	NAME HUDF
Ref:	=2010ApJ...714L..79C
by	CASSATA P. , GIAVALISCO M., GUO Y., FERGUSON H., KOEKEMOER A.M., RENZINI A., FONTANA A., SALIMBENI S., DICKINSON M., CASERTANO S., CONSELICE C.J., GROGIN N., LOTZ J.M., PAPOVICH C., LUCAS R.A., STRAUGHN A., GARDNER J.P., MOUSTAKAS L.
	Astrophys. J., 714L, 79-83 (2010)
	The morphology of passively evolving galaxies at z ~ 2 from Hubble space Telescope/WFC3 deep imaging in the Hubble ultra deep field.
o	Table 1: <[CGG2010] NNNNN> N=6 among (Nos 19389-24626).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGG2011]
[CGG2011]	(Castro+Gizis+Gagne, 2011)
Write:	<<[CGG2011] JHHMMSS.s+DDMMSS>>
N:	25
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of the field of the brown dwarf 2MASS J11395113-3159214.
Ref:	=2011ApJ...736...67C
by	CASTRO P.J. , GIZIS J.E., GAGNE M.
	Astrophys. J., 736, 67 (2011)
	A Chandra observation of the TW Hydrae association brown dwarf 2MASSW J1139511-315921.
o	Table 2: <[CGG2011] JHHMMSS.s+DDMMSS> N=25.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGG2021]
[CGG2021]	(Carlsten+Greene+Greco+, 2021)
Write:	<<[CGG2021] {dw}HHMM{p\|m}DDMM>> <<[CGG2021] dw1044p1351b>> <<[CGG2021] dw1006m0730-n2>>
N:	148+1+1
Object:	Dwarf G (SIMBAD class: Galaxy)
Note:	N=148+1+1 dwarf satellites around 18 host galaxies in the Local Volume (LV). See also [CGB2020], [CGP2020].
Ref:	=2021ApJ...922..267C
by	CARLSTEN S.G. , GREENE J.E., GRECO J.P., BEATON R.L., KADO-FONG E.
	Astrophys. J., 922, 267-267 (2021)
	Structures of dwarf satellites of Milky Way-like galaxies: morphology, scaling relations, and intrinsic shapes.
o	Table 5: <[CGG2021] dwHHMMaDDMM> N=148, <[CGG2021] dw1044p1351b> N=1, <[CGG2021] dw1006m0730-n2> N=1.
=E=	Catalogue in electronic form as <J/ApJ/922/267/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [CGG78]
[CGG78]	(Crampton+Georgelin+Georgelin, 1978)
Write:	<<[CGG78] W 51 a>> <<[CGG78] SNNN Anon>> <<[CGG78] SNNN Anon N>> <<[CGG78] SNNNA Anon>> <<[CGG78] W 58Ga>>
N:	3+21+2
Object:	Region + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 1: N=3 H-alpha regions in W 51 (Nos a-c). Table 2: N=21 stars in the field of 16 HII regions. Text: N=2 possible optical counterpart a and b of W 58G.
in source:	W 51
in source:	W 58:W 58G = W 58G
Ref:	=1978A&A....66....1C
by	CRAMPTON D. , GEORGELIN Y.M., GEORGELIN Y.P.
	Astron. Astrophys., 66, 1-11 (1978)
	First optical detection of W 51 and observations of new H II regions and exciting stars.
o	Table 1: <[CGG78] W 51 a> (Nos a-c). Table 2: <[CGG78] SNNN Anon>, <[CGG78] SNNN Anon N>, <[CGG78] SNNNA Anon>, N=21. Text: <[CGG78] W 58Ga> (Nos 58Ga, 58Gb)>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CGH
CGH	(Chapman+Geller+Huchra)
*****	Avoid the usage of CGH, prefer [CGH87]
Origin	of the Acronym: L (1999A&A...349...97N)
Details on Acronym: CGH-alpha
CGH-alpha	(Castel Gandolfo, H-alpha)
*****	Avoid the usage of CGH-alpha, prefer CGHA
Details on Acronym: CGH-alpha
CGH-alpha	(Cometary Globule, H-alpha)
*****	Avoid the usage of CGH-alpha, prefer [RP93]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CGH2008]
[CGH2008]	(Carrera+Gallart+Hardy+, 2008)
Write:	<<[CGH2008] JHHMMSS.ss+DDMMSS.s>>
N:	626
Object:	RGB* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	CTIO 4m telescope HYDRA spectroscopy to search for Red Giant Branch (RGB) stars in the LMC. See also [CGA2008] in SMC.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2008AJ....135..836C
by	CARRERA R. , GALLART C., HARDY E., APARICIO A., ZINN R.
	Astron. J., 135, 836-849 (2008)
	The chemical enrichment history of the Large Magellanic Cloud.
o	Table 1: <[CGH2008] JHHMMSS.ss+DDMMSS.s> N=626.
=E=	Catalogue in electronic form as J/AJ/135/836
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGH2016]
[CGH2016]	(Cortes+Girart+Hull+, 2016)
Write:	<<[CGH2016] AN>>
N:	15
Object:	Dense Core (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	ALMA band 6 (1mm) observations of N=15 dense cores in the field of [MSL2003] W43-MM1.
in source:	[MSL2003] W43-MM1
Ref:	=2016ApJ...825L..15C
by	CORTES P.C. , GIRART J.M., HULL C.L.H., SRIDHARAN T.K., LOUVET F., PLAMBECK R., LI Z.-Y., CRUTCHER R.M., LAI S.-P.
	Astrophys. J., 825L, 15-15 (2016)
	Interferometric mapping of magnetic fields: the ALMA view of the massive star-forming clump W43-MM1.
o	Fig. 1, Tables 2-3: <[CGH2016] AN> (Nos A, B1-B4, C, D1-D2, E, F1-F2, G-H, J-K).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGH87]
[CGH87]	(Chapman+Geller+Huchra, 1987)= (CGH)
Write:	<<[CGH87] HHMM+DDMMA>>
N:	46+42
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table I: N=47 G in ACO 999, N=46 with 'HHMM+DDMMA' format Table II: N=47 G in ACO 1016, N=42 with 'HHMM+DDMMA' format others galaxies are NGC or IC
in source:	ACO 999
in source:	ACO 1016
Ref:	=1987AJ.....94..571C
by	CHAPMAN G.N.F. , GELLER M.J., HUCHRA J.P.
	Astron. J., 94, 571-586 (1987)
	Linear clusters of galaxies : A 999 and A 1016.
o	some ids are ambiguous. Multiplicity letters may have been added
o	Tables I, II: <[CGH87] HHMM+DDMMA> N=46+42
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGH88]
[CGH88]	(Chapman+Geller+Huchra, 1988)
Write:	<<[CGH88] HHMM+DDMMA>>
N:	214
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Galaxies within 5deg of ACO 194.
Ref:	=1988AJ.....95..999C
by	CHAPMAN G.N.F. , GELLER M.J., HUCHRA J.P.
	Astron. J., 95, 999-1022 (1988)
	Linear clusters of galaxies : A 194.
o	Table I: <[CGH88] HHMM+DDMMA> N=214
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGH94]
[CGH94]	(Cowie+Gardner+Hu+, 1994)= (Hawaii)
Write:	<<[CGH94] SSA NN KNN>>
N:	20+13+12+21
Object:	* + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	In the format, the letter 'K' stands for K-band A colour selected faint object catalogue for Hawaii Deep Survey fields SSA 13 and 22 is found in [CSH96]. (SSA fields are defined in 1991ApJ...369...79L)
Ref:	=1994ApJ...434..114C
by	COWIE L.L. , GARDNER J.P., HU E.M., SONGAILA A., HODAPP K.-W., WAINSCOAT R.J.
	Astrophys. J., 434, 114-127 (1994)
	The Hawaii K-band galaxy survey. I. Deep K-band imaging.
o	<[CGH94] SSA 4 KNN> (Nos 0-19), <[CGH94] SSA 13 KNN> (Nos 0-12), <[CGH94] SSA 17 KNN> (Nos 0-11), <[CGH94] SSA 22 KNN> (Nos 0-20)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGH98]
[CGH98]	(Cooray+Grego+Holzapfel+, 1998)
Write:	<<[CGH98] JHHMM+DDMMA>>
N:	64
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	OVRO and BIMA 28.5GHz continuum observations of N=64 radio-sources identified in 44 galaxy clusters.
Ref:	=1998AJ....115.1388C
by	COORAY A.R. , GREGO L., HOLZAPFEL W.L., JOY M., CARLSTROM J.E.
	Astron. J., 115, 1388-1399 (1998)
	Radio sources in galaxy clusters at 28.5 GHz.
o	Table 3: <[CGH98] JHHMM+DDMMA> N=64.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CGHA
CGHA	(Castel Gandolfo, H-alpha)= (CgH-alpha)
Write:	<<*Em CGHA** NN>>
N:	81
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Ref:	=1976VatOP...1..213M
by	McCARTHY M.F.
	Vatican Obs. Publ., 1, 213-223 (1976)
	Emission Stars in a field in Cyg.
o	Table II: <EM* CGHA NN> (Nos 1-81)
Details on Acronym: [CGI2003]
[CGI2003]	(Cortese+Gavazzi+Iglesias-Paramo+, 2003)
Write:	<<[CGI2003] JHHMMSS+DDMMSS>>
N:	93
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Loiano, Cananea and Calar Alto observations. Optical spectroscopy of 93 galaxies projected in the direction of ACO 1367, Coma Cluster, and Virgo cluster.
in source:	ACO 1367
in source:	Coma Cluster = ACO 1656
in source:	NAME Virgo Cluster
Ref:	=2003A&A...401..471C
by	CORTESE L. , GAVAZZI G., IGLESIAS-PARAMO J., BOSELLI A., CARRASCO L.
	Astron. Astrophys., 401, 471-478 (2003)
	Optical spectroscopy and the UV luminosity function of galaxies in the Abell 1367, Coma and Virgo clusters.
o	Table 2: <[CGI2003] JHHMMSS+DDMMSS> N=60+21+12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGI2005]
[CGI2005]	(Chuprikov+Guirin+Chandra, 2005)
Write:	<<[CGI2005] NN>>
N:	26
Object:	MCQC (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Search for microquasar candidates (MCQC) in a list of ROSAT sources.
Ref:	=2005BaltA..14..446C
by	CHUPRIKOV A. , GUIRIN I., ISHWARA-CHANDRA C.H.
	Baltic Astronomy, 14, 446-450 (2005)
	Low frequency radio observations of microquasar candidates.
o	Table 1: <[CGI2005] NN> (Nos 1-26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGJ2000]
[CGJ2000]	(Coppin+Greaves+Jenness+, 2000) (Not yet in Simbad)
Write:	<<[CGJ2000] +xxx+yyy>>
N:	55
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Note:	N=55 Clumps in OMC 1 region.
in source:	OMC:OMC 1 = OMC 1
Ref:	=2000A&A...356.1031C
by	COPPIN K.E.K. , GREAVES J.S., JENNESS T., HOLLAND W.S.
	Astron. Astrophys., 356, 1031-1038 (2000)
	Structure, star formation and magnetic fields in the OMC1 region.
o	Table 2: <[CGJ2000] +xxx+yyy> N=55.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGJ2011]
[CGJ2011]	(Cognard+Guillemot+Johnson+, 2011)
Write:	<<[CGJ2011] A>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM EPIC observations of the field of PSR J2302+4442.
Ref:	=2011ApJ...732...47C
by	COGNARD I. , GUILLEMOT L., JOHNSON T.J., SMITH D.A., VENTER C., HARDING A.K., WOLFF M.T., CHEUNG C.C., DONATO D., ABDO A.A., BALLET J., CAMILO F., DESVIGNES G., DUMORA D., FERRARA E.C., FREIRE P.C.C., GROVE J.E., JOHNSTON S., KEITH M., KRAMER M., LYNE A.G., MICHELSON P.F., PARENT D., RANSOM S.M., RAY P.S., ROMANI R.W., SAZ PARKINSON P.M., STAPPERS B.W., THEUREAU G., THOMPSON D.J., WELTEVREDE P., WOOD K.S.
	Astrophys. J., 732, 47 (2011)
	Discovery of two millisecond pulsars in Fermi sources with the Nancay radio telescope.
o	Fig. 4: <[CGJ2011] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGJ80]
[CGJ80]	(Canto+Goudis+Johnson+, 1980)
*****	Avoid the usage of [CGJ80], prefer [M77]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGK2006]
[CGK2006]	(Chun+Gharanfoli+Kulkarni+, 2006)
Write:	<<[CGK2006] QSO HHMM+DDd +xx.xx+y.yy>>
N:	1+7+6+5+6+5
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Gemini North NIR AO observations of 6 QSO fields.
Ref:	=2006AJ....131..686C
by	CHUN M.R. , GHARANFOLI S., KULKARNI V.P., TAKAMIYA M.
	Astron. J., 131, 686-700 (2006)
	Adaptive optics imaging of low-redshift damped Lyα quasar absorbers.
o	Table 3: <[CGK2006] QSO HHMM+DDd +XX.xx+Y.yy> N=1+7+6+5+6+5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGK2011]
[CGK2011]	(Clemens+Greiner+Kruehler+, 2011)
Write:	<<[CGK2011] N>> <<[CGK2011] A>>
N:	5+3
Object:	* + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	MPI/ESO 2.2m telescope GROND optical and NIR photometry of N=5 secondary standard stars and N=3 galaxies (including the host galaxy of the GRB) in the field of GRB071028B.
Ref:	=2011A&A...529A.110C
by	CLEMENS C. , GREINER J., KRUEHLER T., PIERINI D., SAVAGLIO S., KLOSE S., AFONSO P.M.J., FILGAS R., OLIVARES F.E., RAU A., SCHADY P., ROSSI A., KUEPCUE YOLDAS A., UPDIKE A.C., YOLDAS A.
	Astron. Astrophys., 529A, 110-110 (2011)
	GRB 071028B, a burst behind large amounts of dust in an unabsorbed galaxy.
o	Table 2: <[CGK2011] N> (Nos 1-5). Figs 1-2, Paragr. 5, Table 3: <[CGK2011] A> (Nos H, G, D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGK94]
[CGK94]	(Cherepashchuk+Goranskij+Karitskaya+, 1994)
Write:	<<[CGK94] KS HHMM+DDd Star N>> <<[CGK94] GRS HHMM+DDd Star N>> <<[CGK94] GRS HHMM.m+DDMM Star N>> <<[CGK94] GRS HHMM+DDd Object N>>
N:	2+2+1+1+5
Object:	* (SIMBAD class: Star)
Note:	Fig.1: N=2 Stars in the field of KS 1731-260 Fig.2: N=2 Stars in the field of KS 1732-273 Fig.5: N=1 Star in the field of GRS 1734-292 (Granat 1734-292) Fig.6: N=1 Star in the field of GRS 1736-297 (Granat 1736-297) Fig.7: N=1 Star in the field of GRS 1741.5-2851 (Granat 1741.5-2851) Fig.8: N=5 Objects in the field of GRS 1747-312 (Granat 1747-312)
Ref:	=1994A&A...289..419C
by	CHEREPASHCHUK A.M. , GORANSKIJ V.P., KARITSKAYA E.A., NADJIP A.E., SAVAGE A., SHAKURA N.I., SUNYAEV R.A., VOLCHKOV A.A.
	Astron. Astrophys., 289, 419-428 (1994)
	The investigation of the error boxes of KVANT and GRANAT X-ray sources in the region of Galactic center.
o	Fig.1: <[CGK94] KS 1731-260 Star N> (Nos 1-2). Fig.2: <[CGK94] KS 1732-273 Star N> (Nos 1-2). Fig.5: <[CGK94] GRS 1734-292 Star N> No. 1. Fig.6: <[CGK94] GRS 1736-297 Star N> No. 1. Fig.7: <[CGK94] GRS 1741.5-2851 Star N> No. 1. Fig.8: <[CGK94] GRS 1747-312 Object N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CGKB
CGKB	(Cool+Grindlay+Krockenberger+Bailyn)
Write:	<<CGKB A>> <<CGKB AN>>
N:	10
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	(Nos A-G) and a group of 3 point sources (C1-C3) ROSAT High Resolution Imager. See also [G93].
in source:	NGC 6397
Ref:	=1993ApJ...410L.103C
by	COOL A.M. , GRINDLAY J.E., KROCKENBERGER M., BAILYN C.D.
	Astrophys. J., 410, 103-106 (1993)
	Discovery of multiple low-luminosity X-ray sources in NGC 6397.
o	<CGKB AN> (Nos A-G, C1-C3).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CGL2003]
[CGL2003]	(Casertano+GOODS Treasury Team+Laidler+, 2003)
Write:	<<[CGL2003] JHHMMSS.ss+DDMMSS.s>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations. Host galaxies of SN 2002KH, SN 2002KI, and SN 2003N.
Ref:	=2003IAUC.8052....1C
by	CASERTANO S. , (The GOODS Treasury Team), LAIDLER V., CAPAK P., COWIE L., (The Hubble Higher-Z Supernova Team), HICKEN M.
	IAU Circ., 8052, 1-None (2003)
	Supernovae 2002kh, 2002ki, and 2003N.
o	<[CGL2003] JHHMMSS.ss+DDMMSS.s> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGL2004]
[CGL2004]	(Caratti o Garatti+Giannini+Lorenzetti+, 2004)
Write:	<<[CGL2004] NNN>>
N:	151
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Observations were carried out with SofI at NTT and ISAAC at VLT. Astrometry and NIR photometry of the star forming region IRAS 08211-4158 in the Vela Molecular Ridge (VMR). New star cluster around IRAS 08211-4158, designated as 'NAME IRAS 08211-4158 CLUSTER', and catalogue of N=151 stars. See also [LLN92], [LGV2002], [MLG99], [MLG2003].
in source:	NAME VMR
Ref:	=2004A&A...422..141C
by	CARATTI O GARATTI A. , GIANNINI T., LORENZETTI D., MASSI F., NISINI B., VITALI F.
	Astron. Astrophys., 422, 141-158 (2004)
	Physical and kinematical properties of a newly discovered star cluster and its associated jet in the Vela Molecular Clouds.
o	Table 2: <[CGL2004] NNN> (Nos 1-151). Table 3: <[LGV2002] IRS 8 ANN> (Nos B0, B8-B13, R0, R7-R9) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGL99]
[CGL99]	(Chuprikov+Girin+Likhachev+, 1999)
Write:	<<[CGL99] NN>>
N:	25
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Pre-launch RadioAstron survey.
Ref:	=1999NewAR..43..747C
by	CHUPRIKOV A.A. , GIRIN I.A., LIKHACHEV S.F., MOLOTOV I.E., DEMENTIEV A.F., LIPATOV B.N., SNEGIREV S.D., MANTOVANI F., TRIGILIO C., ANANTHAKRISHNAN S., BALASUBRAMANIAN V., KULKARNI V.K., SUBRAHMANYA C.R.
	New Astronomy Reviews, 43, 747-750 (1999)
	A pre-launch low frequency VLBI survey for RadioAstron.
o	Table 1: <[CGL99] NN> (Nos 1-25).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGM2012]
[CGM2012]	(Clarkson+Ghez+Morris+, 2012)
Write:	<<[CGM2012] NNN>>
N:	432
Object:	* (SIMBAD class: Star)
Note:	Keck NIRC2 observations of N=432 stars in the Arches cluster.
in source:	NAME Arches Cluster
Ref:	=2012ApJ...751..132C
by	CLARKSON W.I. , GHEZ A.M., MORRIS M.R., LU J.R., STOLTE A., McCRADY N., DO T., YELDA S.
	Astrophys. J., 751, 132 (2012)
	Proper motions of the Arches cluster with Keck Laser Guide Star Adaptive Optics: the first kinematic mass measurement of the Arches.
o	(Erratum) erratum vol. 753, art. 92 (2012)
o	Table 5: <[CGM2012] NNN> (Nos 1-432).
=E=	Catalogue in electronic form as J/ApJ/751/132
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGM90]
[CGM90]	(Carico+Graham+Matthews+, 1990)
Write:	<<[CGM90] IRAS HHMMm+DDMM WW>> <<[CGM90] IRAS HHMMm+DDMM W>>
N:	8
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=4 double nuclei IRAS galaxies, the 2 nuclei are designated by their positions 'W' or 'WW'.
in source:	IRAS 08572+3915
in source:	IRAS 12112+0305
in source:	IRAS 14348-1447
in source:	IRAS 22491-1808
Ref:	=1990ApJ...349L..39C
by	CARICO D.P. , GRAHAM J.R., MATTHEWS K., WILSON T.D., SOIFER B.T., NEUGEBAUER G., SANDERS D.B.
	Astrophys. J., 349, 39-42 (1990)
	The near-infrared morphology of ultraluminous infrared galaxies.
o	Table 1: <[CGM90] IRAS HHMMm+DDMM WW>, <[CGM90] IRAS HHMMm+DDMM W>, N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGM97]
[CGM97]	(Colina+Garcia Vargas+Mas-Hesse+, 1997)
Write:	<<[CGM97] NGC NNNN Core>> <<[CGM97] NGC NNNN A>> <<[CGM97] NGC NNNN ANN>>
N:	20+20
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations In NGC 4303: N=1 'Core', N=12 star-forming regions (Nos A-L), N=7 regions among (Nos R10 -R40) In 3351: N=1 'Core', N=11 star-forming regions (Nos A-K), N=8 regions among (Nos R20-R75)
in source:	NGC 4303
in source:	NGC 3351
Ref:	=1997ApJ...484L..41C
by	COLINA L. , GARCIA-VARGAS M.L., MAS-HESSE J.M., ALBERDI A., KRABBE A.
	Astrophys. J., 484, 41-46 (1997)
	Nuclear spiral and ring star-forming structures and the starburst-active galactic nucleus connection in barred spirals NGC 3351 and NGC 4303.
o	Table 1: <[CGM97] NGC 4303 Core> N=1, <[CGM97] NGC 4303 A> (Nos A-K), <[CGM97] NGC 4303 RNN> N=7 among (Nos R10 -R40). Table 2: <[CGM97] NGC 3351 Core> N=1, <[CGM97] NGC 3351 A> (Nos A-K), <[CGM97] NGC 3351 RNN> N=8 among (Nos R20-R75).
Ref:	=2002ApJ...579..545C
by	COLINA L. , GONZALEZ-DELGADO R., MAS-HESSE J.M., LEITHERER C.
	Astrophys. J., 579, 545-553 (2002)
	Detection of a super-star cluster as the ionizing source in the low-luminosity active galactic nucleus NGC 4303.
o	(Erratum) Errata vol. 582, p. 1269 (2003) ; vol. 586, p. 692 (2003)
o	Table 1: <[CGM97] NGC 4303 A> (No. L) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CGMW
CGMW	(Candidate G behind the Milky Way)= (CGMW1) = (CGMW2) = (CGMW3) = (CGMW4) = (CGMW5) = (Sait)
Write:	<<CGMW 1-NNNN>> <<CGMW 2-NNNN>> <<CGMW 3-NNNNa>> <<CGMW 4-NNNN>> <<CGMW 5-NNNNN>>
N:	2411+4633+5332+7154+11310
Object:	G (SIMBAD class: Galaxy)
Note:	List 1: format '1-NNNN', N=2411 List 2: format '2-NNNN', N=4633 List 3: format '3-NNNN', N=5332 and '3-NNNNa', N=2 components for the H-alpha emission line of No. 4360 (a and b) List 4: format '4-NNNN', N=7154 List 5: format '5-NNNNN', N=11310. Catalogues are compiled in a database.
Ref:	=1990PASJ...42..603S
by	SAITO M. , OHTANI H., ASONUMA A., KASHIKAWA N., MAKI T., NISHIDA S., WATANABE T.
	Publ. Astron. Soc. Jap., 42, 603-None (1990)
	A search for galaxies behind the Milky Way between l=210°. and 230°.
o	Table 5: IRAS 07384-0344 misprint for 07387-0344
o	<CGMW 1-NNNN> (Nos 1-1 to 1-2411) (here table 5: N=81)
Ref:	=1991PASJ...43..449S
by	SAITO M. , OHTANI H., BABA A., HOTTA H., KAMENO S., KUROSU S., NAKADA K., TAKATA T.
	Publ. Astron. Soc. Jap., 43, 449-468 (1991)
	A search for galaxies behind the Milky Way between l = 230 °. and 250 °.
o	IRAS 06477-2713 misprint for 06447-271
o	<CGMW 2-NNNN> (Nos 2-1 to 2-4633) (here table 4: N=232)
Ref:	=1996PASJ...48..679R
by	ROMAN A.T. , NAKANISHI K., TOMITA A., SAITO M.
	Publ. Astron. Soc. Jap., 48, 679-690 (1996)
	A search for galaxies behind the Milky Way at Aquila and Sagittarius.
o	<CGMW 3-NNNN> (Nos 3-1 to 3-5332) (here table 5: N=104). Table 8: <[RNT96] ClG N> (Nos 1-2).
Ref:	=1998PASJ...50...47R
by	ROMAN A.T. , TAKEUCHI T.T., NAKANISHI K., SAITO M.
	Publ. Astron. Soc. Jap., 50, 47-54 (1998)
	A redshift survey for galaxies behind the Milky Way near the Galactic Center.
o	Table 1: <CGMW 3-NNNNa> N=2 components
Ref:	=1998PASJ...50...37R
by	ROMAN A.T. , NAKANISHI K., SAITO M.
	Publ. Astron. Soc. Jap., 50, 37-46 (1998)
	A systematic search for galaxies behind the Milky Way at Sagittarius.
o	<CGMW 4-NNNN> (Nos 4-1 to 4-7154) (here table 2: N=107)
Ref:	=2000ApJS..127...27R
by	ROMAN A.T. , IWATA I., SAITO M.
	Astrophys. J., Suppl. Ser., 127, 27-38 (2000)
	A visual search for galaxies in a Milky Way region around the North Supergalactic Pole.
o	Table 2: <CGMW 5-NNNNN> N=11310.
=E=	Catalogue in electronic form as VII/209
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CGMW1
CGMW1	(Candidate G behind the Milky Way, Vol.1)
*****	Avoid the usage of CGMW1, prefer CGMW
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CGMW2
CGMW2	(Candidate G behind the Milky Way, Vol.2)
*****	Avoid the usage of CGMW2, prefer CGMW
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CGMW3
CGMW3	(Candidate G behind the Milky Way, Vol.3)
*****	Avoid the usage of CGMW3, prefer CGMW
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CGMW4
CGMW4	(Candidate G behind the Milky Way, Vol.4)
*****	Avoid the usage of CGMW4, prefer CGMW
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CGMW5
CGMW5	(Candidate G behind the Milky Way, Vol.5)
*****	Avoid the usage of CGMW5, prefer CGMW
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CGN2006]
[CGN2006]	(Caratti o Caratti+Giannini+Nisini+, 2006) (Not yet in Simbad)
Write:	<<[CGN2006] VLA 1623 A>>
N:	4
Object:	(Near IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Near-IR outflows: the first composed of 2 knots A and B, the second of bow shocks C and D in AMDM VLA 1623.4-2418.
in source:	NAME rho Oph Cloud
Ref:	=2006A&A...449.1077C
by	CARATTI O GARATTI A. , GIANNINI T., NISINI B., LORENZETTI D.
	Astron. Astrophys., 449, 1077-1088 (2006)
	H_{2} active jets in the near IR as a probe of protostellar evolution.
o	Fig.11, Table 7: <[DE95] NGC 2264G AN> (Nos I1-I5, H1-H5) added. Fig.12, Table 7: <[CGN2006] VLA 1623 A> (Nos A-D). Fig.12, Table 7: <[GSWC2003] NNa> (Nos 14h, 14i, 17b) added. Fig.17, Table 7: <[NMV2001] Knot A> (Nos N-R) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGN93]
[CGN93]	(Caswell+Gardner+Norris+, 1993)
*****	Avoid the usage of [CGN93], prefer Caswell
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGN99]
[CGN99]	(Cappa+Goss+Niemela+, 1999)
Write:	<<[CGN99] NN>> <<[CGN99] A>>
N:	13+5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=13 small-diameter radio continuum sources in the field of NGC 2359 (Nos 1-13). Fig.4: N=5 HI filaments (Nos A-E) in NGC 2359. See also [CRG2001].
in source:	NGC 2359
Ref:	=1999AJ....118..948C
by	CAPPA C.E. , GOSS W.M., NIEMELA V.S., OSTROV P.G.
	Astron. J., 118, 948-959 (1999)
	A study of neutral and ionized gas of the Wolf-Rayet ring nebula NGC 2359.
o	Table 2: <[CGN99] NN> (Nos 1-13). Fig.4: <[CGN99] A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CGO
CGO	(Catalog of Gal. O *)
Write:	<<CGO NNN>>
N:	664
Object:	O * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1974RMxAA...1..211C
by	CRUZ-GONZALEZ C. , RECILLAS-CRUZ E., COSTERO R., PEIMBERT M., TORRES-PEIMBERT S.
	Rev. Mex. Astron. Astrofis., 1, 211-259 (1974)
	A catalogue of galactic O stars. The ionization of the low density interstellar medium by runaway stars.
o	in ref list ANDREWS MmRAS.72.35 instead of MNRAS.72.35
o	Table 1: <CGO NNN> (Nos 1-664)
=E=	Catalogue in electronic form as III/84
=E=	Catalogue in electronic form as <III/84B/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CGP2011]
[CGP2011]	(Corbelli+Giovanardi+Palla+, 2011)= ([CGP2011a])
Write:	<<[CGP2011] sNN>>
N:	20
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	IRAM 30m CO line observations of N=20 sources in M 33.
in source:	M 33 = NGC 598
Ref:	=2011A&A...528A.116C
by	CORBELLI E. , GIOVANARDI C., PALLA F., VERLEY S.
	Astron. Astrophys., 528A, 116-116 (2011)
	On the nature of faint mid-infrared sources in M33.
o	Tables 1-6: <[CGP2011] sNN> (Nos s1-s20).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGP2011a]
[CGP2011a]	(Corbelli+Giovanardi+Palla+, 2011)
*****	Avoid the usage of [CGP2011a], prefer [CGP2011]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGP2011b]
[CGP2011b]	(Chapman+goldsmith+Pineda+, 2011)
Write:	<<[CGP2011b] JHHMMSS.s+DDMMSS>>
N:	125+162
Object:	* (SIMBAD class: Star)
Note:	H band polarization measurements with the Mimir instrument at the 1.8m Perkins telescope (Flagstaff) in the region of the Taurus molecular cloud.
in source:	NAME Taurus Cloud
Ref:	=2011ApJ...741...21C
by	CHAPMAN N.L. , GOLDSMITH P.F., PINEDA J.L., CLEMENS D.P., LI D., KRCO M.
	Astrophys. J., 741, 21 (2011)
	The magnetic field in Taurus probed by infrared polarization.
o	Tables 1-2: <[CGP2011b] JHHMMSS.s+DDMMSS> N=125+162.
=E=	Catalogue in electronic form as J/ApJ/741/21
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGP2016]
[CGP2016]	(Castelletti+Giacani+Petriella, 2016)
Write:	<<[CGP2016] Cloud A>> <<[CGP2016] Cloud>>
N:	4 (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	JCMT HARP-ACSIS CO(3-2) observations of the field of SNR G011.0-00.0.
in source:	HESS J1809-193
in source:	SNR G011.0-00.0
Ref:	=2016A&A...587A..71C
by	CASTELLETTI G. , GIACANI E., PETRIELLA A.
	Astron. Astrophys., 587A, 71-71 (2016)
	Unveiling the origin of HESS J1809-193.
o	Table 2: <[CGP2016] Cloud> N=1, <[CGP2016] Cloud A> N=3 (A, B and C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGP2020]
[CGP2020]	(Carlsten+Greene +Peter+, 2020)
Write:	<<[CGP2020] dwHHMMpDDMM>>
N:	4
Object:	Dwarf G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=2+2 satellites around M101 and NGC 4631 respectively. Use of DECALS data. See also [CGB2020] and [CGG2021].
in source:	NGC 5457 = M 101
in source:	NGC 4631
Ref:	=2020ApJ...902..124C
by	CARLSTEN S.G. , GREENE J.E., PETER A.H.G., GRECO J.P., BEATON R.L.
	Astrophys. J., 902, 124-124 (2020)
	Radial distributions of dwarf satellite systems in the Local Volume.
o	Table 1: <[CGP2020] dwHHMMpDDMM> N=4.
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: CGPG
CGPG	(Compact Galaxies and Post-eruptive Galaxy)= (ZGC)
Write:	<<CGPG HHMM.m+DDMM>>
N:	>3700
Object:	G (SIMBAD class: Galaxy)
Note:	Most of the objects in this catalogue were originally published in the seven first lists of 'Zw R NNN'. Ex.: 'CGPG 0000.6+2142' = Zw IV 1 This catalogue is known as the 'Red Book'. See also Zw.
Ref:	=1971CGPG..C......0Z
by	ZWICKY F.
	Publ. F. Zwicky, Guemligen (BE), Switzerland, 0-388 (1971)
	Catalogue of selected compact galaxies and of post-eruptive galaxies.
o	<CGPG HHMM.m+DDMM> N about 3700. <Zw R NNNa> R from (Nos I to VII).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CGPS
CGPS	(Canadian Galactic Plane Survey)
Write:	<<CGPS JHHMMSS+DDMMSS>>
N:	72787
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Catalog of compact sources of radio emission at 1420MHz in the northern Galactic plane from the Canadian Galactic Plane Survey.
Ref:	=2017AJ....153..113T
by	TAYLOR A.R. , LEAHY D.A., TIAN W.W., SUNSTRUM C., KOTHES R., LANDECKER T.L., RANSOM R.R., HIGGS L.A.
	Astron. J., 153, 113-113 (2017)
	A 1420 MHz catalog of compact sources in the northern Galactic plane.
o	Table 2: <CGPS JHHMMSS+DDMMSS> N=72787.
=E=	Catalogue in electronic form as <J/AJ/153/113/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CGPS
CGPS	(Canadian Galactic Plane Survey)
Write:	<<CGPS LLL.ll+B.bb>>
N:	380
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	DRAO observations. N=380 compact extragalactic sources in the Galactic Plane.
Ref:	=2003ApJS..145..213B
by	BROWN J.C. , TAYLOR A.R., JACKEL B.J.
	Astrophys. J., Suppl. Ser., 145, 213-223 (2003)
	Rotation measures of compact sources in the Canadian galactic plane survey.
o	Table 1: <CGPS LLL.ll+B.bb> N=380.
=E=	Catalogue in electronic form as J/ApJS/145/213
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CGPSE
CGPSE	(Canadian Galactic Plane Survey, Extended source)
Write:	<<CGPSE NNN>>
N:	201
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	New catalogue of extended radio sources at 1420 and 408MHz using the DRAO interferometer.
Ref:	=2007MNRAS.379..289K
by	KERTON C.R. , MURPHY J., PATTERSON J.
	Mon. Not. R. Astron. Soc., 379, 289-296 (2007)
	A sharper view of the outer Galaxy at 1420 and 408 MHz from the Canadian Galactic Plane Survey II: the catalogue of extended radio sources.
o	Table 1: <CGPSE NNN> (Nos 1-201).
=E=	Catalogue in electronic form as J/MNRAS/379/289
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CGR-F
CGR-F	(Compact Group of Radio-sources in FIRST)
Write:	<<CGR-F JHHMMSS.s+DDMMSS>>
N:	35
Object:	Group of Radios (SIMBAD class: Radio = Radio Source)
Note:	Search for groups of radio-sources from the FIRST catalog. See also 5GR.
Ref:	=2003AstL...29..224G
by	GUBANOV A.G. , KOPYLOV A.I., POTAPOV A.S.
	Astron. Lett., 29, 224-235 (2003)
	Search for groups of extragalactic radio sources.
o	Table: <5GR NNNN.NN> N=35 = <CGR-F JHHMMSS.s+DDMMSS> N=35.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CGR2017]
[CGR2017]	(Chanchaiworawit+Guzman+Rodriguez Espinosa+, 2017)= ([CGR2017a])
Write:	<<[CGR2017] LAE-C-N-NN>>
N:	47
Object:	Poss. LAE G (SIMBAD class: EmObj = Emission Object)
Note:	GTC OSIRIS observations of N=2 spectroscopically confirmed LAEs and N=45 other LAE candidates in the SXDS field.
in source:	NAME SXDSF
Ref:	=2017MNRAS.469.2646C
by	CHANCHAIWORAWIT K. , GUZMAN R., RODRIGUEZ ESPINOSA J.M., CASTRO-RODRIGUEZ N., SALVADOR-SOLE E., CALVI R., GALLEGO J., HERRERO A., MANRIQUE A., MARIN-FRANCH A., MAS-HESSE J.M., ARETXAGA I., CARRASCO E., TERLEVICH E., TERLEVICH R.
	Mon. Not. R. Astron. Soc., 469, 2646-2661 (2017)
	Gran Telescopio Canarias observations of an overdense region of Lyman α emitters at z = 6.5.
o	Table 2: <[CGR2017] LAE-C-N-NN> (Nos 1-01 to 1-15, 2-16 to 2-47).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGR2017a]
[CGR2017a]	(Chanchaiworawit+Guzman+Rodriguez Espinosa+, 2017)
*****	Avoid the usage of [CGR2017a], prefer [CGR2017]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGR2017b]
[CGR2017b]	(Caminha+Grillo+Rosati+, 2017)
Write:	<<[CGR2017b] MACS J0416 NNa>>
N:	37+114
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	N=37 systems of N=114 gravitationally lensed images in the MCS J0416.1-2403 gravitational lens system. Use of archival MUSE data and of CLASH-VLT data.
in source:	MCS J0416.1-2403
Ref:	=2017A&A...600A..90C
by	CAMINHA G.B. , GRILLO C., ROSATI P., BALESTRA I., MERCURIO A., VANZELLA E., BIVIANO A., CAPUTI K.I., DELGADO-CORREAL C., KARMAN W., LOMBARDI M., MENEGHETTI M., SARTORIS B., TOZZI P.
	Astron. Astrophys., 600A, 90-90 (2017)
	A refined mass distribution of the cluster MACS J0416.1-2403 from a new large set of spectroscopic multiply lensed sources.
o	Catalog: <CLASHVLT JHHMMSS.ss+DDMMSS.s> N=4594. Fig. 1, Table A.1: <[CGR2017b] MACS J0416 NNa> (Nos 1-37, 1a-1c to 37a-37c).
=E=	Catalogue in electronic form as <J/A+A/600/A90/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGR2017c]
[CGR2017c]	(Caminha+Grillo+Rosati+, 2017)
Write:	<<[CGR2017c] MACS J1206 NN>> <<[CGR2017c] MACS J1206 NNa>>
N:	27+85+14
Object:	G + Grav. lensed image of a G + Poss. Grav. lensed image of a G (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy)
Note:	VLT MUSE observations of N=85 gravitationally lensed images and N=14 predicted images of N=27 background sources, lensed by the cluster MCS J1206.2-0847. Use of CLASH (HST) and CLASH-VLT (VLT VIMOS) data.
in source:	MCS J1206.2-0847
Ref:	=2017A&A...607A..93C
by	CAMINHA G.B. , GRILLO C., ROSATI P., MENEGHETTI M., MERCURIO A., ETTORI S., BALESTRA I., BIVIANO A., UMETSU K., VANZELLA E., ANNUNZIATELLA M., BONAMIGO M., DELGADO-CORREAL C., GIRARDI M., LOMBARDI M., NONINO M., SARTORIS B., TOZZI P., BARTELMANN M., BRADLEY L., CAPUTI K.I., COE D., FORD H., FRITZ A., GOBAT R., POSTMAN M., SEITZ S., ZITRIN A.
	Astron. Astrophys., 607A, 93-93 (2017)
	Mass distribution in the core of MACS J1206. Robust modeling from an exceptionally large sample of central multiple images.
o	Figs 1+A.1, Table A.1: <[CGR2017c] MACS J1206 NN> (Nos 1-27), <[CGR2017c] MACS J1206 NNa> N=85+14 among (Nos 1a-1c to 27a-27c).
o	G1 not identified
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGR2018]
[CGR2018]	(Cantiello+Grado+Rejkuba+, 2018)
Write:	<<[CGR2018] NNN>>
N:	347
Object:	Poss. GlCl + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	ESO VST and VISTA high-resolution observations of N=347 globular cluster candidates in NGC 253.
in source:	NGC 253
Ref:	=2018A&A...611A..21C
by	CANTIELLO M. , GRADO A., REJKUBA M., ARNABOLDI M., CAPACCIOLI M., GREGGIO L., IODICE E., LIMATOLA L.
	Astron. Astrophys., 611A, 21-21 (2018)
	A VST and VISTA study of globular clusters in NGC 253.
o	Table 3: <[CGR2018] NNN> (Nos 1-347).
=E=	Catalogue in electronic form as J/A+A/611/A21
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CGRaBS
CGRaBS	(Candidate Gammay-Ray Blazar Survey)
Write:	<<CGRaBS JHHMM+DDMM>>
N:	1625
Object:	Poss. Blazar (SIMBAD class: AGN = Active Galaxy Nucleus)
Stat:	is completely incorporated in Simbad
Note:	Catalog of radio-loud AGNs and QSOs based on X-ray (ROSAT) and radio (CRATES) fluxes.
Ref:	=2008ApJS..175...97H
by	HEALEY S.E. , ROMANI R.W., COTTER G., MICHELSON P.F., SCHLAFLY E.F., READHEAD A.C.S., GIOMMI P., CHATY S., GRENIER I.A., WEINTRAUB L.C.
	Astrophys. J., Suppl. Ser., 175, 97-104 (2008)
	CGRaBS: an all-sky survey of γ-ray blazar candidates.
o	Catalog: <CGRaBS JHHMM+DDMM> N=1625.
=E=	Catalogue in electronic form as J/ApJS/175/97
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CGRO
CGRO	(Compton Gamma Ray Observatory)
Origin	of the Acronym: L (1996MNRAS.282L..33B)
Details on Acronym: [CGS2015]
[CGS2015]	(Chengalur+Ghosh+Salter+, 2013)
Write:	<<[CGS2015] N>>
N:	4
Object:	HI (SIMBAD class: HI = HI (21cm) Source)
Note:	VLA HI observations of N=4 emitters in the field of PG 1216+069. Use of archival VLA data.
Ref:	=2015MNRAS.453.3135C
by	CHENGALUR J.N. , GHOSH T., SALTER C.J., KANEKAR N., MOMJIAN E., KEENEY B.A., STOCKE J.T.
	Mon. Not. R. Astron. Soc., 453, 3135-3142 (2015)
	HI 21cm emission from the subdamped Lyman-α absorber at z = 0.0063 towards PG 1216+069.
o	Fig. 3, Table 2: <[CGS2015] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CGSS
CGSS	(Catalog of Galactic S Star)
*****	Avoid the usage of CGSS, prefer CSS
Origin	of the Acronym: L (1986IAUC.4225....0W)
Details on Acronym: [CGV2000]
[CGV2000]	(Corradi+Goncalves+Villaver+, 2000) (Not yet in Simbad)
Write:	<<[CGV2000] NGC 6337 A>> <<[CGV2000] He 2-186 A>> <<[CGV2000] IC 2553 A>> <<[CGV2000] IC 2553 A'>>
N:	3+2
Object:	Feature (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	1st ref.: Fig.1: N=3 bright filaments in NGC 6337. Fig.5: N=2 bright elongated knots in Hen 2-186. 2nd ref.: Figs 1, 2: Knots in pair (AA', BB', CC') in IC 2553, located symmetrically with respect to the central star.
in source:	NGC 6337
in source:	Hen 2-186
in source:	IC 2553
Ref:	=2000ApJ...535..823C
by	CORRADI R.L.M. , GONCALVES D.R., VILLAVER E., MAMPASO A., PERINOTTO M., SCHWARZ H.E., ZANIN C.
	Astrophys. J., 535, 823-832 (2000)
	High-velocity collimated outflows in planetary nebulae: NGC 6337, He 2-186, and K4-47.
o	Fig.1: <[CGV2000] NGC 6337 A> (Nos A-C). Fig.5: <[CGV2000] He 2-186 A> (Nos A-B).
Ref:	=2000ApJ...542..861C
by	CORRADI R.L.M. , GONCALVES D.R., VILLAVER E., MAMPASO A., PERINOTTO M.
	Astrophys. J., 542, 861-869 (2000)
	Knots in the outer shells of the planetary nebulae IC 2553 and NGC 5882.
o	Figs 1, 2: <[CGV2000] IC 2553 A> (Nos A-C), <[CGV2000] IC 2553 A'> (Nos A'-C').
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGV2010]
[CGV2010]	(Carrasco+Gomez+Verdugo+, 2010)
Write:	<<[CGV2010] AN>> <<[CGV2010] A.N>> (not recognised by Simbad, but found in literature)
N:	10+1
Object:	G + Grav. lensed image (SIMBAD class: Galaxy)
Note:	Gemini South GMOS observations of the core of the nearby cluster Abell 3827.
in source:	ACO 3827
Ref:	=2010ApJ...715L.160C
by	CARRASCO E.R. , GOMEZ P.L., VERDUGO T., LEE H., DIAZ R., BERGMANN M., TURNER J.E.H., MILLER B.W., WEST M.J.
	Astrophys. J., 715L, 160-164 (2010)
	Strong gravitational lensing by the super-massive cD galaxy in Abell 3827.
o	Fig. 1, Table 1: <[CGV2010] AN> (Nos N1-N5, A1-A4, B1).
Ref:	=2015MNRAS.449.3393M
by	MASSEY R. , WILLIAMS L., SMIT R., SWINBANK M., KITCHING T.D., HARVEY D., JAUZAC M., ISRAEL H., CLOWE D., EDGE A., HILTON M., JULLO E., LEONARD A., LIESENBORGS J., MERTEN J., MOHAMMED I., NAGAI D., RICHARD J., ROBERTSON A., SAHA P., SANTANA R., STOTT J., TITTLEY E.
	Mon. Not. R. Astron. Soc., 449, 3393-3406 (2015)
	The behaviour of dark matter associated with four bright cluster galaxies in the 10 kpc core of Abell 3827.
o	Table 3: <[CGV2010] N6> added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGV2014]
[CGV2014]	(Cummings+Geisler+Villanova+, 2014) (Not yet in Simbad)
Write:	<<[CGV2014] NNNNN>>
N:	18460
Object:	* (SIMBAD class: Star)
Note:	LCO 1-m Swope telescope observations of N=14860 stars in the globular cluster NGC 1851.
in source:	NGC 1851
Ref:	=2014AJ....148...27C
by	CUMMINGS J.D. , GEISLER D., VILLANOVA S., CARRARO G.
	Astron. J., 148, 27 (2014)
	Uncovering multiple populations with Washington photometry. I. The globular cluster NGC 1851.
o	Table 2: <[CGV2014] NNNNN> (Nos 2-18461).
=E=	Catalogue in electronic form as <J/AJ/148/27/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGW2001]
[CGW2001]	(Conselice+Gallagher+Wyse, 2001) (Not yet in Simbad)
Write:	<<[CGW2001] Filament NN>> <<[CGW2001] Cluster NN>> <<[CGW2001] Arm AN>>
N:	38+22+2
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
in source:	NGC 1275 = 3C 84
Ref:	=2001AJ....122.2281C
by	CONSELICE C.J. , GALLAGHER III J.S., WYSE R.F.G.
	Astron. J., 122, 2281-2300 (2001)
	On the nature of the NGC 1275 system.
o	Fig.5, Table 1: <[CGW2001] Filament NN> (Nos 1-38). Fig.9, Table 2: <[CGW2001] Cluster NN> (Nos 1-22), <[CGW2001] Arm AN> (Nos A1-A2). Fig. 3: <NAME Perseus Horseshoe>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGW2003]
[CGW2003]	(Conselice+Gallagher+Wyse, 2003)
Write:	<<[CGW2003] NN>> <<[CGW2003] JHHMMSS.s+DDMM>>
N:	53
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Sample of Low-Mass Cluster Galaxies in the Perseus Cluster.
in source:	NAME Perseus Cluster
Ref:	=2003AJ....125...66C
by	CONSELICE C.J. , GALLAGHER III J.S., WYSE R.F.G.
	Astron. J., 125, 66-85 (2003)
	Galaxy populations and evolution in clusters. III. The origin of low-mass galaxies in clusters: constraints from stellar populations.
o	Table 1: <[CGW2003] NN> (Nos 1-53) = <[CGW2003] JHHMMSS.s+DDMM> N=53.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGW2012]
[CGW2012]	(Ciardullo+Gronwall+Wolf+, 2012)
Write:	<<[CGW2012] NNN>>
N:	199 (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	CTIO Blanco 4 m telescope MOSAIC II CCD camera narrow-band observations of the Chandra Deep Field-South.
in source:	NAME Chandra Deep Field-South
Ref:	=2012ApJ...744..110C
by	CIARDULLO R. , GRONWALL C., WOLF C., McCATHRAN E., BOND N.A., GAWISER E., GUAITA L., FELDMEIER J.J., TREISTER E., PADILLA N., FRANCKE H., MATKOVIC A., ALTMANN M., HERRERA D.
	Astrophys. J., 744, 110 (2012)
	The evolution of lyα-emitting galaxies between z = 2.1 and z = 3.1.
o	Tables 2-3: <[CGW2012] NNN> N=199.
=E=	Catalogue in electronic form as <J/ApJ/744/110/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CGW2013]
[CGW2013]	(Cassata+Giavalisco+Williams+, 2013)
Write:	<<[CGW2013] NNN>>
N:	107 (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	CANDELS observations of N=107 passive early-type galaxies (ETGs) in the GOODS-S field.
in source:	NAME GOODS Southern Field
Ref:	=2013ApJ...775..106C
by	CASSATA P. , GIAVALISCO M., WILLIAMS C.C., GUO Y., LEE B., RENZINI A., FERGUSON H., FABER S.F., BARRO G., McINTOSH D.H., LU Y., BELL E.F., KOO D.C., PAPOVICH C.J., RYAN R.E., CONSELICE C.J., GROGIN N., KOEKEMOER A., HATHI N.P.
	Astrophys. J., 775, 106 (2013)
	Constraining the assembly of normal and compact passively evolving galaxies from redshift z = 3 to the present with CANDELS.
o	Table 1: <[CGW2013] NNN> (Nos 1-107).
=E=	Catalogue in electronic form as <J/ApJ/775/106/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CH
CH	(Campbell+Hunter+)
*****	Avoid the usage of CH, prefer [CHH92]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Ch
Ch	(Chiron)
*****	Avoid the usage of Ch, prefer Chiron
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Ch
Ch	(Chincarini+)
*****	Avoid the usage of Ch, prefer [CTB81]
Origin	of the Acronym: L (1995ApJS...96..343Q)
Details on Acronym: CH
CH	(Carbon, Hydrogen)
*****	Avoid the usage of CH, prefer [HC88]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Ch
Ch	(Chamaeleon DCld)
*****	Avoid the usage of Ch, prefer [VMF94]
Origin	of the Acronym: L (1999ApJS..123..233L)
Details on Acronym: [CH2001]
[CH2001]	(Challis+High-z supernovae search team, 2001)= ([CH2001a])
Write:	<<[CH2001] JHHMMSS.ss+DDMMSS.s>>
N:	2
Object:	Poss. SN + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST WFPC2 observations. N=1 probable SN and N=1 elongated faint galaxy.
Ref:	=2001IAUC.7668....1C
by	CHALLIS P. , (The High-Z Supernova Search Team)
	IAU Circ., 7668, 1-None (2001)
	Probable supernova in anonymous galaxy.
o	<[CH2001] JHHMMSS.ss+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CH2001a]
[CH2001a]	(Challis+High-z supernovae search team, 2001)
*****	Avoid the usage of [CH2001a], prefer [CH2001]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CH2001b]
[CH2001b]	(Corral+Herrero, 2001)
Write:	<<[CH2001b] NN>>
N:	48
Object:	Poss. PN (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=48 candidate PN in the Southern arm of M 33.
in source:	M 33 = NGC 598
Ref:	=2001A&A...376..820C
by	CORRAL L.J. , HERRERO A.
	Astron. Astrophys., 376, 820-824 (2001)
	Planetary nebula candidates in a southern region of M 33.
o	Table 3: <[CH2001b] NN> (Nos 1-48).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CH2005a]
[CH2005a]	(Cioni+Habing, 2005)
Write:	<<[CH2005a] DDD.dddddd+DD.dddddd>>
N:	9374+16354
Object:	(Near IR) * (SIMBAD class: Star)
Note:	NIR observations with the 4.2m WHT on La Palma of NGC 6822.
in source:	NGC 6822
Ref:	=2005A&A...429..837C
by	CIONI M.-R.L. , HABING H.J.
	Astron. Astrophys., 429, 837-850 (2005)
	Near-IR observations of NGC 6822: AGB stars, distance, metallicity and structure.
o	Tables 1, 2: <[CH2005a] DDD.dddddd+DD.dddddd> N=9374+16354.
=E=	Catalogue in electronic form as J/A+A/429/837
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CH2005b]
[CH2005b]	(Cioni+Habing, 2005)
Write:	<<[CH2005b] DDD.dddddd+DD.dddddd>>
N:	2570
Object:	(Near IR) * (SIMBAD class: Star)
Note:	NIR observations with the 4.2m WHT on La Palma of Draco Dwarf Galaxy.
in source:	NAME Draco Dwarf Galaxy
Ref:	=2005A&A...442..165C
by	CIONI M.-R.L. , HABING H.J.
	Astron. Astrophys., 442, 165-176 (2005)
	The Draco dwarf galaxy in the near-infrared.
o	Table 1: <[CH2005b] DDD.dddddd+DD.dddddd> N=2570.
=E=	Catalogue in electronic form as J/A+A/442/165
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CH2010]
[CH2010]	(Cody+Hillenbrand, 2010)
Write:	<<[CH2010] CTIO JHHMMSSss+DDMMSSs>>
N:	8
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	CTIO 1.0m telescope observations of N=8 variable stars in the field of the σ Orionis cluster.
in source:	NAME sig Ori Cluster
Ref:	=2010ApJS..191..389C
by	CODY A.M. , HILLENBRAND L.A.
	Astrophys. J., Suppl. Ser., 191, 389-422 (2010)
	Precision photometric monitoring of very low mass σ Orionis cluster members: variability and rotation at a few Myr.
o	Table 3: <[CH2010] CTIO JHHMMSSss+DDMMSSs> N=8.
=E=	Catalogue in electronic form as J/ApJS/191/389
Details on Acronym: [CH2017]
[CH2017]	(Caglar+Hudaverdi, 2017)
Write:	<<[CH2017] A3653W>>
N:	2
Object:	Subcluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	N=2 sub-clusters in the galaxy cluster ACO 3653. Use of AAT, Chandra, and XMM-Newton archival data.
in source:	ACO 3653
Ref:	=2017MNRAS.472.2633C
by	CAGLAR T. , HUDAVERDI M.
	Mon. Not. R. Astron. Soc., 472, 2633-2642 (2017)
	Dynamical history of a binary cluster: Abell 3653.
o	Fig. 2: <[CH2017] A3653W> (Nos A3653E, A3653EW).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CH2018]
[CH2018]	(Chen+Hirano, 2018)
Write:	<<[CH2018] VLA 1623-NN>> <<[CH2018] SM1-W>>
N:	2+1
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	SMA 1.3mm observations of N=2+1 millimeter sources in the ρ Oph A ridge. Use of SMA, IRAM 30m, and JCMT archival data.
in source:	NAME rho Oph A
in source:	WRW rho Oph SM 1
in source:	AMDM VLA 1623.0-2418 = NAME VLA 1623
Ref:	=2018ApJ...868...80C
by	CHEN Y.-C. , HIRANO N.
	Astrophys. J., 868, 80-80 (2018)
	The physical and chemical properties of the ρ Ophiuchi A dense core.
o	Fig. 1, Table 1: <[CH2018] VLA 1623-NN> (Nos N1-N2), <[CH2018] SM1-W> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CH69]
[CH69]	(Cudaback+Heiles, 1969)
Write:	<<[CH69] GLLL.l+BB.b>>
N:	81
Object:	Cloud (SIMBAD class: Cloud)
Note:	Hat Creek 85-ft radio telescope observations of N=81 interstellar dust clouds.
Ref:	=1969ApJ...155L..21C
by	CUDABACK D.D. , HEILES C.
	Astrophys. J., 155L, 21 (1969)
	A survey of dust clouds for OH emission.
o	Table 1: <[CH69] GLLL.l+BB.b> N=81.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CH79]
[CH79]	(Cudworth+Herbig, 1979)
Write:	<<[CH79] A>>
N:	1
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=1 star in the field of SSV LDN 1551 5, HH 28 and HH 29.
Ref:	=1979AJ.....84..548C
by	CUDWORTH K.M. , HERBIG G.
	Astron. J., 84, 548-551 (1979)
	Two large-proper-motion Herbig-Haro objects.
o	Table II: <Em* LkHA NNN> (Nos 358-359) added. Table II: <[CH79] A> (No. A).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CH87]
[CH87]	(Caswell+Haynes, 1987)= ([CH87a])
Write:	<<[CH87] LLL.lll+B.bbb>>
N:	311
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Ref:	=1987A&A...171..261C
by	CASWELL J.L. , HAYNES R.F.
	Astron. Astrophys., 171, 261-276 (1987)
	Southern HII regions: an extensive study of radio recombination line emission.
o	<[CH87] LLL.lll+B.bbb> N=311
=E=	Catalogue in electronic form as J/A+A/171/261
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CH87a]
[CH87a]	(Caswell+Haynes, 1987)
*****	Avoid the usage of [CH87a], prefer [CH87]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CH87b]
[CH87b]	(Colless+Hewett, 1987)
Write:	<<[CH87b] CNN NN>> <<[CH87b] AC1 NN>>
N:	687
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	G in 14 clusters, 13 numbered among Nos (C02 to C67) from a preliminary version of the southern cluster survey of Abell + Corwin, unpublished. A 14th cluster is numbered as 'AC1' by the authors. Tables 3a: G in C02 = ACO 2717: 'CO2 NN', (Nos 1-50) Tables 3b: G in C03 = ACO 2721: 'CO3 NN', (Nos 1-47) Tables 3c: G in C19 = ACO 3126: 'C19 NN', (Nos 1-50) Tables 3d: G in C20 = DRCG 0329-52: 'C20 NN', (Nos 1-50) Tables 3e: G in C21 = ACO 458: 'C21 NN', (Nos 1-50) Tables 3f: G in AC1 = Str 0409-597: 'AC1 NN', (Nos 1-50) Tables 3g: G in C30 = ACO 3334: 'C30 NN', (Nos 1-48) Tables 3h: G in C31 = ACO 3360: 'C31 NN', (Nos 1-48) Tables 3i: G in C37 = ACO 3705: 'C37 NN', (Nos 1-50) Tables 3j: G in C39 = ACO S 906: 'C39 NN', (Nos 1-48) Tables 3k: G in C52 = ACO 3854: 'C52 NN', (Nos 1-48) Tables 3l: G in C64 = ACO 2538: 'C64 NN', (Nos 1-50) Tables 3m: G in C65 = ACO 2554: 'C65 NN', (Nos 1-48) Tables 3n: G in C67 = Braid 272: 'C67 NN', (Nos 1-50)
in source:	ACO 2717
in source:	ACO 2721
in source:	ACO 3126
in source:	DRCG 0329-52
in source:	ACO 458
in source:	ACO 3225
in source:	ACO 3334
in source:	ACO 3360
in source:	ACO 3705
in source:	ACO S 906
in source:	ACO 3854
in source:	ACO 2538
in source:	ACO 2554
in source:	ACO S 1157
Ref:	=1987MNRAS.224..453C
by	COLLESS M. , HEWETT P.
	Mon. Not. R. Astron. Soc., 224, 453-472 (1987)
	The dynamics of rich clusters - I. Velocity data.
o	Tables 3a to 3n: <[CH87b] CNN NN>, <[CH87b] AC1 NN> N=687
=E=	Catalogue in electronic form as J/MNRAS/224/453
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ch90
Ch90	(Chambers+, 1990)
Write:	<<Ch90 4C 41.17 AN>> <<Ch90 a>> <<Ch90 A>>
N:	7+7
Object:	(Rad) + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Radio components of 4C.17, format '4C 41.17 AN'. Objects in the field: format 'a' or 'A', (Nos v-z, A) In component 'N' the letter N stands for Nucleus See also [CMV96]
Ref:	=1990ApJ...363...21C
by	CHAMBERS K.C. , MILEY G.K., VAN BREUGEL W.J.M.
	Astrophys. J., 363, 21-39 (1990)
	4C 41.17: a radio galaxy at a redshift of 3.8.
o	Table 2: <Ch90 4C 41.17 AN> (Nos A, B1-B3, C). Table 4: <Ch90 a> (Nos v-z), <Ch90 A> No. A
Ref:	=1994AJ....107..480C
by	CARILLI C.L. , OWEN F.N., HARRIS D.E.
	Astron. J., 107, 480-493 (1994)
	Radio continuum polarimetric imaging of high redshift radio galaxies.
o	(Erratum) erratum AJ 107 p. 2299
o	Table 2: <Ch90 4C 41.17 A> No. N added. Table 3: <[COH94] 0902+343 AN> (Nos A1-A2, B1-B2, J1-J2, N>
Ref:	=2002ApJ...569..611S
by	STEINBRING E. , CRAMPTON D., HUTCHINGS J.B.
	Astrophys. J., 569, 611-623 (2002)
	Radio galaxies at z = 1.1 to 3.8: adaptive optics imaging and archival Hubble Space Telescope data.
o	Table 4, Figs 1 to 5: <[SCH2002] 3C 356 aN> (Nos a-b, a1-a2), <[SCH2002] 3C 230 a> (Nos a-c), <[SCH2002] 3C 230 N> (No. 1), <[SCH2002] 3C 68.2 a> (Nos a-b), <[SCH2002] 3C 68.2 N> (Nos 1-3), <[SCH2002] 3C 294 a> (Nos a-d), <[SCH2002] 3C 294 N> (Nos 1-2), <[SCH2002] TXS 0828+193 a> (Nos a-e), <[SCH2002] TXS 0828+193 N> (No. 1). Table 4, Fig.6: <Ch90 4C 41.17 AN> (Nos A1, A2) added.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CH94]
[CH94]	(Campbell-Wilson+Hunstead, 1994)= (MOST)
Write:	<<[CH94] HHMM+DDd>>
N:	55
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Ref:	=1994PASAu..11...33C
by	CAMPBELL-WILSON D. , HUNSTEAD R.W.
	Proc. Astron. Soc. Australia, 11, 33-38 (1994)
	Variable radio sources at 843 MHz.
o	<[CH94] HHMM-DDd> N=55
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CH96]
[CH96]	(Cohen+Hitchon, 1996)
Write:	<<[CH96] AFGL 2881 N>>
N:	2
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Note:	The authors designate these 2 stars as 'GL 2881 N'. '[CH96] AFGL 2881 1' = 'AFGL 2881', '[CH96] AFGL 2881 2' is associated with IRAS 22165+4331
Ref:	=1996AJ....111..962C
by	COHEN M. , HITCHON K.
	Astron. J., 111, 962-969 (1996)
	Studies of extreme carbon stars. II. Periods from optical spectral characteristics.
o	obj. 'GL NNNN' = 'AFGL NNNN'
o	'GL 2881 N' use <[CH96] AFGL 2881 N> (Nos 1-2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CH98]
[CH98]	(Cowie+Hu, 1998)
Write:	<<[CH98] HDF LA N>> <<[CH98] SSA 22 LA N>>
N:	5+7
Object:	Em. Obj. (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Table 1: Lyman Alpha (LA) emitting objects in HDF and SSA 22 fields.
Ref:	=1998AJ....115.1319C
by	COWIE L.L. , HU E.M.
	Astron. J., 115, 1319-1328 (1998)
	High-z Ly-α emitters. I. A blank-field search for objects near redshift z = 3.4 in and around the Hubble Deep Field and the Hawaii deep field SSA 22.
o	Table 1: <[CH98] HDF LA N> (Nos 1-5), <[CH98] SSA 22 LA N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CHA
CHA	(Center for High Ambular resolution)
*****	Avoid the usage of CHA, prefer CHR
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Cha
Cha	(Chamaeleon)
*****	Avoid the usage of Cha, prefer Ass Cha T
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Cha
Cha	(Chamaeleon)
*****	Avoid the usage of Cha, prefer Ass Cha T
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CHa
CHa	(CDF-S Halpha)
*****	Avoid the usage of CHa, prefer [FRM2009]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cha
Cha	(Chamaeleon)
*****	Avoid the usage of Cha, prefer HJM
Origin	of the Acronym: L (1994MNRAS.268....1W)
Details on Acronym: Cha
Cha	(Chamaeleon)= (Cha)
*****	Avoid the usage of Cha, prefer [L2007b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cha
Cha	(Chamaeleon)
Write:	<<NAME Cha N>>
N:	2
Object:	Dark Cloud (SIMBAD class: Cloud)
Ref:	=1977ApJS...35..161S
by	SCHWARTZ R.D.
	Astrophys. J., Suppl. Ser., 35, 161-170 (1977)
	A survey of southern dark clouds for Herbig-Haro objects and H alf emission stars.
o	Table 2: <HH NN> (Nos 44-57). Tables 3-9: <Sz NNN> (Nos 1-140). Tables 5-8: <Lupus N> (Nos 1-4). <NAME Cha N> (Nos 1-2). <NAME Norma DCLD>.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cha
Cha	(Chamaeleon)
*****	Avoid the usage of Cha, prefer [NC98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cha
Cha	(Chavira)
*****	Avoid the usage of Cha, prefer Ton
Details on Acronym: Cha
Cha	(Chamaeleon DCld)
*****	Avoid the usage of Cha, prefer [VMF94]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Cha
Cha	(Chamaeleon)
*****	Avoid the usage of Cha, prefer WKK
Origin	of the Acronym: L (1994MNRAS.268....1W)
Details on Acronym: [CHA90]
[CHA90]	(Couture+Harris+Allwright, 1990)
Write:	<<[CHA90] NNN>>
N:	273
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
in source:	M 87 = NGC 4486 = Virgo A
Ref:	=1990ApJS...73..671C
by	COUTURE J. , HARRIS W.E., ALLWRIGHT J.W.B.
	Astrophys. J., Suppl. Ser., 73, 671-683 (1990)
	BVI photometry of globular clusters in M 87.
o	<[CHA90] NNN> N=273
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHA91]
[CHA91]	(Couture+Harris+Allwright, 1991)
Write:	<<[CHA91] NGC 4472 NNN>> <<[CHA91] NGC 4649 NNN>>
N:	230+296
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	Table 2: format 'NGC 4472 NNN', N=230 GlCl in NGC 4472 Table 3: format 'NGC 4649 NNN',N=296 GlCl in NGC 4649.
in source:	NGC 4472 = M 49
in source:	NGC 4649
Ref:	=1991ApJ...372...97C
by	COUTURE J. , HARRIS W., ALLWRIGHT J.W.B.
	Astrophys. J., 372, 97-110 (1991)
	Multicolor CCD photometry of globular clusters in two Virgo elliptical galaxies.
o	Table 2: <[CHA91] NGC 4472 NNN> N=230. Table 3: <[CHA91] NGC 4649 NNN> N=296
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ChaG
ChaG	(Chavira, G)
*****	Avoid the usage of ChaG, prefer [C89]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: ChaHalpha
ChaHalpha	(Chamaeleon, H-alpha)
*****	Avoid the usage of ChaHalpha, prefer [NC98]
Origin	of the Acronym: L (2004A&A...416..555L)
Details on Acronym: ChaI
ChaI	(Chamaeleon I)
*****	Avoid the usage of ChaI, prefer [LES2004]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ChaII
ChaII	(Chamaeleon II)
*****	Avoid the usage of ChaII, prefer [LEM2005b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cham
Cham	(Chamaeleon)
*****	Avoid the usage of Cham, prefer HJM
Origin	of the Acronym: L (1997ApJ...489..719M)
Details on Acronym: ChaMP
ChaMP	(Chandra Multiwave Plane survey)
*****	Avoid the usage of ChaMP, prefer [ZGH2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CHARA
CHARA	(Center for High Ambular Resolution Astronomy)
*****	Avoid the usage of CHARA, prefer CHR
Origin	of the Acronym: L (1996AJ....112.2260M)
Details on Acronym: Chariklo
Chariklo	(10199 Chariklo occult.) (Not yet in Simbad)
Write:	<<Chariklo 10199-NNN>>
N:	117
Object:	* (SIMBAD class: Star)
Ref:	=2000AJ....119.2008S
by	STONE R.C. , McDONALD S.W., ELLIOT J.L., BOWELL E.
	Astron. J., 119, 2008-2017 (2000)
	10199 Chariklo stellar occultation candidates: 1999-2005.
o	Table 4: <Chariklo 10199-NNN> (Nos 1-117).
=E=	Catalogue in electronic form as J/AJ/119/2008
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Charon
Charon	(Charon occult.)= (C)
Write:	<<Charon NNN>> <<Charon NNN.NN>>
Object:	* (SIMBAD class: Star)
Note:	Events are numbered sequentially in time, 'NNN' Nos among (Nos 10-659). The authors have 'interpolated' decimal values '.NN' for events falling chronologically between events 'NNN' Those stars occulted by both Charon and Pluto have the same number.
Ref:	=1991AJ....101.2255M
by	MINK D.J. , KLEMOLA A.R., BUIE M.W.
	Astron. J., 101, 2255-2261 (1991)
	Occultations by Pluto and Charon: 1990-1999.
o	Table 1: <Pluto NN> N=32 among (Nos 10-49). Table 2: <Charon NN> N=28 among (Nos 10-49)
Ref:	=1991AJ....102.1464D
by	DUNHAM E.W. , McDONALD S.W., ELLIOT J.L.
	Astron. J., 102, 1464-1484 (1991)
	Pluto-Charon stellar occultation candidates: 1990-1995.
o	Table 2: <Pluto NN.NN> N=59 new inclusions. Table 3: <Charon NN.NN> N=60 new inclusions.
Ref:	=1996AJ....112..788M
by	McDONALD S.W. , ELLIOT J.L.
	Astron. J., 112, 788-796 (1996)
	Pluto-Charon stellar occultation candidates 1996-1999.
o	Table 2: <Pluto NN.NN> N=52 new inclusions. Table 3: <Charon NN.NN> N=56 new inclusions
Ref:	=2000AJ....119.1999M
by	McDONALD S.W. , ELLIOT J.L.
	Astron. J., 119, 1999-2007 (2000)
	Pluto-Charon stellar occultation candidates: 2000-2009.
o	(Erratum) Erratum vol. 120, p. 1599 (2000)
o	Table 2: <Pluto NNN> N=486 among (Nos 50-659). Table 3: <Charon NNN> N=479 among (Nos 50-659).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ChASeM33
ChASeM33	(Chandra ACIS Survey of M 33)
Write:	<<ChASeM33 NNN>> <<ChASeM33 JHHMMSS.ss+DDMMSS.s>>
N:	394+662
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS Survey of M 33. 2008ApJS..174..366P: Format NNN (Nos 1-394), for the sources in the "first look" catalogue. 2011ApJS..193...31T: Format JHHMMSS.ss+DDMMSS.s, for the N=662 sources in the final catalogue.
in source:	M 33 = NGC 598
Ref:	=2008ApJS..174..366P
by	PLUCINSKY P.P. , WILLIAMS B., LONG K.S., GAETZ T.J., SASAKI M., PIETSCH W., TULLMANN R., SMITH R.K., BLAIR W.P., HELFAND D., HUGHES J.P., WINKLER P.F., DE AVILLEZ M., BIANCHI L., BREITSCHWERDT D., EDGAR R.J., GHAVAMIAN P., GRINDLAY J., HABERL F., KIRSHNER R., KUNTZ K., MAZEH T., PANNUTI T.G., SHPORER A., THILKER D.A.
	Astrophys. J., Suppl. Ser., 174, 366-378 (2008)
	Chandra ACIS survey of M33 (ChASeM33): a first look.
o	Table 2: <ChASeM33 NNN> (Nos 1-394).
Ref:	=2011ApJS..193...31T
by	TULLMANN R. , GAETZ T.J., PLUCINSKY P.P., KUNTZ K.D., WILLIAMS B.F., PIETSCH W., HABERL F., LONG K.S., BLAIR W.P., SASAKI M., WINKLER P.F., CHALLIS P., PANNUTI T.G., EDGAR R.J., HELFAND D.J., HUGHES J.P., KIRSHNER R.P., MAZEH T., SHPORER A.
	Astrophys. J., Suppl. Ser., 193, 31 (2011)
	The Chandra ACIS survey of M33 (ChASeM33): the final source catalog.
o	Tables 3-7, 9: <ChASeM33 JHHMMSS.ss+DDMMSS.s> N=662.
=E=	Catalogue in electronic form as J/ApJS/174/366
=E=	Catalogue in electronic form as J/ApJS/193/31
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Chavira
Chavira	(Chavira)
*****	Avoid the usage of Chavira, prefer Ton
Details on Acronym: [CHB2000]
[CHB2000]	(Cohen+Hogg+Blandford+, 2000)
Write:	<<[CHB2000] {H\|F\|O}MMSS.ss-MMSS.s>>
N:	671
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Format: offset position relative to RA=12h, Dec=+62 deg. In the format the letter 'H' stands for (HDF fields), 'F' (Flanking field) or 'O' (Outside). See also [HPA2000], [C2001b]. In ref. 2001AJ....121.2895C Tables 6A, 6B, additional redshifts for some galaxies.
in source:	NAME HDFN
Ref:	=2000ApJ...538...29C
by	COHEN J.G. , HOGG D.W., BLANDFORD R., COWIE L.L., HU E., SONGAILA A., SHOPBELL P., RICHBERG K.
	Astrophys. J., 538, 29-52 (2000)
	Caltech faint galaxy redshift survey. X. A redshift survey in the region of the Hubble Deep Field North.
o	Table 7: 'CHHMMS_MMSS' and 'PHHMMS_MMSS' are '[HPA2000] JHHMMSS.ss+DDMMSS.s' objects, 'VHHMMS_MMSS' are '[RKF98] MMSS+MMSS' objects, with rounded formats in this table.
o	Table 2a: <[CHB2000] FMMSS.ss-MMSS.s> N=510. Table 2b: <[CHB2000] HMMSS.ss-MMSS.s> N=146. Table 2c: <[CHB2000] OMMSS.ss-MMSS.s> N=15.
=E=	Catalogue in electronic form as J/ApJ/538/29
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ChCl
ChCl	(Choi, Clump)
Write:	<<ChCl A>>
N:	2
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=2 Clumps in HH 170-110 region. See also ChMM.
in source:	NAME HH 270-110
Ref:	=2001ApJ...550..817C
by	CHOI M.
	Astrophys. J., 550, 817-823 (2001)
	Observations of molecular clouds in the HH 270/110 region.
o	Table 1, Fig.1: <ChMM N> (Nos 1-2). Fig.4: <ChCl A> (Nos A-B).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CHF2011]
[CHF2011]	(Cockcroft+Harris+Ferguson+, 2011)
Write:	<<[CHF2011] M33 S>>
N:	1
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	CFHT MegaCam observations of M33.
in source:	M 33 = NGC 598
Ref:	=2011ApJ...730..112C
by	COCKCROFT R. , HARRIS W.E., FERGUSON A.M.N., HUXOR A., IBATA R., IRWIN M.J., McCONNACHIE A.W., WOODLEY K.A., CHAPMAN S.C., LEWIS G.F., PUZIA T.H.
	Astrophys. J., 730, 112 (2011)
	The M33 globular cluster system with PAndAS data: the last outer halo cluster?
o	Cluster S is [SVA2008] M 33-EC1 in SIMBAD.
o	Fig. 1, Tables 3-4: <[HFB2009] HM33-A> (No. E) added, <[CHF2011] M33 S> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHG2004]
[CHG2004]	(Christensen+Hjorth+Gorosabel+, 2004)
Write:	<<[CHG2004] A>> <<[CHG2004] N>>
N:	4+6
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Image of GRB 990712 field: secondary standards in the field. See also [SVB2000].
Ref:	=2004A&A...413..121C
by	CHRISTENSEN L. , HJORTH J., GOROSABEL J., VREESWIJK P., FRUCHTER A., SAHU K., PETRO L.
	Astron. Astrophys., 413, 121-130 (2004)
	The host galaxy of GRB 990712.
o	Fig.1, Table1: <[CHG2004] A> (Nos A-D), <[CHG2004] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHG2008]
[CHG2008]	(Castro+Herrero+Garcia+, 2008)
Write:	<<[CHG2008] A-NN>> <<[CHG2008] CN-NN>>
N:	339+21+36+39+33
Object:	Blue * (SIMBAD class: Star)
Note:	ESO VLT FORS2 observations of NGC 55.
in source:	NGC 55
Ref:	=2008A&A...485...41C
by	CASTRO N. , HERRERO A., GARCIA M., TRUNDLE C., BRESOLIN F., GIEREN W., PIETRZYNSKI G., KUDRITZKI R.-P., DEMARCO R.
	Astron. Astrophys., 485, 41-50 (2008)
	The Araucaria Project: VLT-spectroscopy of blue massive stars in NGC55.
o	Table A1: <[CHG2008] A-NN> N=39 among (Nos 1-45), <[CHG2008] B-NN> N=21 among (Nos 3-37), <[CHG2008] C1-NN> N=36 among (Nos 1-52), <[CHG2008] C2-NN> N=39 among (Nos 1-55),<[CHG2008] D-NN> N=33 among (Nos 1-46).
=E=	Catalogue in electronic form as J/A+A/485/41
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHG2019]
[CHG2019]	(Cortes+Hull+Girart+, 2019)
Write:	<<[CHG2019] W43-MMN A>>
N:	81
Object:	Core (SIMBAD class: denseCore = Dense Core)
Note:	ALMA Band 6 (1.3mm) observations of N=81 cores in 6 clumps in W 43. See also [CGH2016].
in source:	W 43
Ref:	=2019ApJ...884...48C
by	CORTES P.C. , HULL C.L.H., GIRART J.M., ORQUERA-ROJAS C., SRIDHARAN T.K., LI Z.-Y., LOUVET F., CORTES J.R., LE GOUELLEC V.J.M., CRUTCHER R.M., LAI S.-P.
	Astrophys. J., 884, 48-48 (2019)
	The seven most massive clumps in W43-Main as seen by ALMA: dynamical equilibrium and magnetic fields.
o	Table 3: <[CHG2019] W43-MMN A> N=81.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHG85]
[CHG85]	(Castelaz+Hackwell+Grasdalen+, 1985)= (IRS) = ([WKG93])
Write:	<<[CHG85] IRS N>>
N:	4
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	GSS 30
Ref:	=1985ApJ...290..261C
by	CASTELAZ M.W. , HACKWELL J.A., GRASDALEN G.L., GEHRZ R.D., GULLIXSON C.
	Astrophys. J., 290, 261-272 (1985)
	GSS 30 : an infrared reflection nebula in the Ophiuchus dark cloud.
o	(Erratum) + erratum vol. 301, 502
o	Table 1: <[CHG85] GSS 30 IRS N> (Nos 1-2)
Ref:	=1993AJ....105..271W
by	WEINTRAUB D.A. , KASTNER J.H., GRIFFITH L.L., CAMPINS H.
	Astron. J., 105, 271-283 (1993)
	Near-infrared, polarimetric imaging of the bipolar lobes of GSS 30: protostellar infall and/or outflow?
o	Table 1: [WKG93] use <[CHG85] IRS N> (Nos 1-4) Nos 3-4 are new
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHG99]
[CHG99]	(Carlson+Holtzman+Grillmair+, 1999) (Not yet in Simbad)
Write:	<<[CHG99] xxx.xx-yyy.yy>>
N:	5
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST WFPC2 images of NGC 3597. N=5 star clusters.
in source:	NGC 3597
Ref:	=1999AJ....117.1700C
by	CARLSON M.N. , HOLTZMAN J.A., GRILLMAIR C.J., MOULD J.R., GRIFFITHS R.E., BALLESTER G.E., BURROWS C.J., CLARKE J.T., CRISP D., EVANS R.W., GALLAGHER III J.S., HESTER J.J., HOESSEL J.G., SCOWEN P.A., STAPELFELDT K.R., TRAUGER J.T., WATSON A.M., WESTPHAL J.A.
	Astron. J., 117, 1700-1707 (1999)
	Deep Hubble Space Telescope observations of blue star clusters in NGC 3597.
o	Table 1: <[CHG99] xxx.xx-yyy.yy> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHH2006]
[CHH2006]	(Choi+Hodapp+Hayashi+, 2006)
Write:	<<[CHH2006] NNa>>
N:	21
Object:	H2 feature (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	NGC 1333 region H2 emission obtained using the QUIRC camera at the UH2.2m telescope.
in source:	NGC 1333:[JCC87] IRAS 4 = [JCC87] IRAS 4
Ref:	=2006ApJ...646.1050C
by	CHOI M. , HODAPP K.W., HAYASHI M., MOTOHARA K., PAK S., PYO T.-S.
	Astrophys. J., 646, 1050-1058 (2006)
	Variability of the NGC 1333 IRAS 4A outflow: molecular hydrogen and silicon monoxide images.
o	Table 1: <[CHH2006] NNa> (Nos 1-4, 5a-5c, 6-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHH92]
[CHH92]	(Campbell+Hunter+Holtzman+, 1992)= (CH) = (WF)
Write:	<<[CHH92] NNN>> <<[CHH92] NNNN>>
N:	214+801
Object:	* (SIMBAD class: Star)
Note:	Table 2: (Nos 1-214), stars in RMC 136 Tables 3, 4, 5, 6: stars outside RMC 136 Table 3: (Nos 5001-5104), Table 4: (Nos 6001-6477), Table 5: (Nos 7001-7162), Table 6: (Nos 8001-8058), first digit 5 to 8 for * found on PC5 to 8.
in source:	Magellanic Clouds:LMC:RMC 136 = RMC 136
Ref:	=1992AJ....104.1721C
by	CAMPBELL B. , HUNTER D.A., HOLTZMAN J.A., LAUER T.R., SHAYA E.J., CODE A., FABER S.M., GROTH E.J., LIGHT R.M., LYNDS R., O'NEIL E.J.Jr, WESTPHAL J.A.
	Astron. J., 104, 1721-1742 (1992)
	Hubble-Space Telescope planetary camera images of R136.
o	Plate 115, Fig. 2: <RMC 136aNN> N=24 Table 2: <[CHH92] NNN> (Nos 1-214), Table 3: <[CHH92] 5NNN> (Nos 5001-5104), Table 4: <[CHH92] 6NNN> (Nos 6001-6477), Table 5: <[CHH92] 7NNN> (Nos 7001-7162), Table 6: <[CHH92] 8NNN> (Nos 8001-8058)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHI2010]
[CHI2010]	(Currie+Hernandez+Irwin+, 2010)
Write:	<<[CHI2010] PNNNNN>> <<[CHI2010] SNNNNN>> <<[CHI2010] NNNN>> <<[CHI2010] h Per MNNNNN>> <<[CHI2010] chi Per MNNNN>>
N:	40760+11309+7465+13424+4720
Object:	* (SIMBAD class: Star)
Note:	Photometry (KPNO Mayall Mosaic Imager) and spectroscopy (MMT Hectospec, WIYN Hydra, FLWO FAST) of the Double Cluster h and chi Persei.
in source:	h Per Cluster = NGC 869
in source:	chi Per Cluster = NGC 884
Ref:	=2010ApJS..186..191C
by	CURRIE T. , HERNANDEZ J., IRWIN J., KENYON S.J., TOKARZ S., BALOG Z., BRAGG A., BERLIND P., CALKINS M.
	Astrophys. J., Suppl. Ser., 186, 191-221 (2010)
	The stellar population of h and χ Persei: cluster properties, membership, and the intrinsic colors and temperatures of stars.
o	Table 1: <[CHI2010] PNNNNN> (Nos P1-P47060). Table 2: <[CHI2010] SNNNNN> (Nos S1-S11309). Table 3: <[CHI2010] NNNN> (Nos 1-7465). Table 6: <[CHI2010] h Per MNNNNN> (Nos M1-M13424), <[CHI2010] χ Per MNNNNN> (Nos M1-M4720).
=E=	Catalogue in electronic form as <J/ApJS/186/191/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHI90]
[CHI90]	(Cristiani+Hawkins+Iovino+, 1990)
Write:	<<[CHI90] QHHMM+DDMMA>> <<[CHI90] HHMM+DDMMA>>
N:	29
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=26 QSO, format 'QHHMM+DDMMA' and N=3 stars or galaxy, format 'HHMM+DDMMA'.
Ref:	=1990MNRAS.245..493C
by	CRISTIANI S. , HAWKINS M., IOVINO A., PIERRE M., SHAVER P.
	Mon. Not. R. Astron. Soc., 245, 493-502 (1990)
	Observations of variable quasar candidates.
o	Table 1: <[CHI90] QHHMM+DDMMA> N=26, <[CHI90] HHMM+DDMMA> N=3
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CHIIXR
CHIIXR	(Chamaeleon II, X-ray source, ROSAT satellite)
Write:	<<CHIIXR NN>>
N:	40
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT PSPC observations of Chamaeleon II dark cloud. See also XHXR.
in source:	NAME Cha II
Ref:	=2000A&A...355..629A
by	ALCALA J.M. , COVINO E., STERZIK M.F., SCHMITT J.H.M.M., KRAUTTER J., NEUHAEUSER R.
	Astron. Astrophys., 355, 629-638 (2000)
	A ROSAT pointed observation of the Chamaeleon II dark cloud.
o	Table 1: <CHIIXR NN> (Nos 1-40).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CHIMPS
CHIMPS	(CO Heterodyne Inner MilkyWay Plane Survey)
Write:	<<CHIMPS NNNN>> <<CHIMPS GLLL.lll+BB.bbb>>
N:	4999
Object:	Clump (SIMBAD class: MolCld = Molecular Cloud)
Note:	JCMT HARP 330GHz observations of N=4999 13CO(3-2) clumps in the inner Galactic Plane, as part of the CO Heterodyne Inner Milky Way Plane Survey (CHIMPS). Use of 12CO(3-2) data from the CO High Resolution Survey (COHRS).
Ref:	=2019A&A...632A..58R
by	RIGBY A.J. , MOORE T.J.T., EDEN D.J., URQUHART J.S., RAGAN S.E., PERETTO N., PLUME R., THOMPSON M.A., CURRIE M.J., PARK G.
	Astron. Astrophys., 632A, 58-58 (2019)
	CHIMPS: physical properties of molecular clumps across the inner Galaxy.
o	Tables 1+4: <CHIMPS NNNN> (Nos 0001-4999) = <CHIMPS GLLL.lll+BB.bbb> N=4999.
=E=	Catalogue in electronic form as <J/A+A/632/A58/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Chini
Chini	(Chini)
*****	Avoid the usage of Chini, prefer [C81]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ChIPS
ChIPS	(Champlane Infrared Plane Survey)
Write:	<<ChIPS JHHMMSS.ss+DDMMSS.s>>
N:	1000000
Object:	* (SIMBAD class: Star)
Note:	ChaMPlane is a multiwavelength survey. This catalog (ChIPS) of Infrared sources will join our X-ray catalog CXOPS and our optical catalog ChOPS. Preliminary references: 2003AN....324...57G, 2003AN....324..176Z.
Notes:	The Chandra Multiwavength Plane (ChaMPlane) Survey of the galactic plane incorporates serendipitous sources from selected Chandra pointings in or near the galactic plane (b < 12deg, >20 ksec, lack of bright diffuse or point sources) to measure or constrain the luminosity function of low-luminosity accretion sources in the Galaxy. The primary goal is to detect and identify accreting white dwarfs (cataclysmic variables, with space density still uncertain by a factor of >10-100), neutron stars and black holes (quiescent low mass X-ray binaries) to constrain their space densities and thus origin and evolution. Secondary objectives are to identify Be stars in high mass X-ray binaries and constrain their space densities, and to survey the H-R diagram for stellar coronal sources. A parallel optical imaging under the NOAO Long Term Survey program provides deep optical images using the Mosaic imager on the CTIO and KPNO 4-m telescopes. The 36x36arcmin optical images (Halpha, R, V and I) cover 5X the area of each enclosed Chandra ACIS FOV, providing an extended survey of emission line objects for comparison with Chandra. Spectroscopic followup of optical counterparts is then conducted, thus farwith WIYN and Magellan. In the highly obscured fields in the PLane and toward the Galactic Center, an infrared survey is being made, to identify the X-ray sources that cannot be detected at optical wavelengths. This catalog contains all ChaMPlane Infrared point sources, their positions, J,H,Ks magnitudes and links to probable counterparts in our X-ray and optical catalogs. http://hea-www.harvard.edu/ChaMPlane
Auth.:	GRINDLAY J.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CHIPS
CHIPS	(Clusters Hiding in Plain Sight)
*****	Avoid the usage of CHIPS, prefer [SMG2021]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Chiron
Chiron	(Chiron)= (Ch)
Write:	<<Chiron NN>>
N:	91
Object:	* (SIMBAD class: Star)
Ref:	=1994AJ....107.1814B
by	BUS S.J. , WASSERMAN L.H.
	Astron. J., 107, 1814-1824 (1994)
	Chiron stellar occultation candidates: 1993-1996.
o	<Chiron NN> N=44
Ref:	=1996AJ....112.1683P
by	PERSON M.J. , BUS S.J., WASSERMAN L.H., ELLIOT J.L.
	Astron. J., 112, 1683-1689 (1996)
	Chiron stellar occultation candidates 1996-2000.
o	Table 2: <Chiron NN> (Nos 45-91)
=E=	Catalogue in electronic form as J/AJ/107/1814
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Chiu
Chiu	(Chiu)= (KC)
Write:	<<Chiu SA 51 NNN>> <<Chiu SA 57 NNN>> <<Chiu SA 68 NNN>>
N:	567+188+216
Object:	* (SIMBAD class: Star)
Note:	Table 6: format 'SA 51 NNN', N=567 * in SA 51 Table 7: format 'SA 57 NNN', N=188, * in SA 58 Table 8: format 'SA 68 NNN', N=216, * in SA 68
in source:	SA 51-
in source:	SA 57-
in source:	SA 68-
Ref:	=1980ApJS...44...31C
by	CHIU L.-T.G.
	Astrophys. J., Suppl. Ser., 44, 31-71 (1980)
	Classification of stellar populations and luminosity classes from accurate proper motions .
o	Cross-id. not in Simbad
o	Table 6: <Chiu SA 51 NNN> N=567. Table 7: <Chiu SA 57 NNN> N=188. Table 8: <Chiu SA 68 NNN> N=216
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CHK2004]
[CHK2004]	(Chini+Hoffmeister+Kampgen+, 2004)
Write:	<<[CHK2004] KW N>>
N:	2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT ISAAC infrared observations of KW object. The object is resolved into a system of two early B-type stars.
in source:	NAME Kleinmann-Wright Object
Ref:	=2004A&A...427..849C
by	CHINI R. , HOFFMEISTER V.H., KAEMPGEN K., KIMESWENGER S., NIELBOCK M., SIEBENMORGEN R.
	Astron. Astrophys., 427, 849-853 (2004)
	The nature of the KW object.
o	Fig.1, Table 1: <[CHK2004] KW N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHL2002]
[CHL2002]	(Coe+Haigh+Laycock+, 2002) (Not yet in Simbad)
Write:	<<[CHL2002] NNN>>
N:	4
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Fig.1: Finding chart of AX J0051-733. Four objects numbered 476, 499, 512 and 647 are in the error circle and possible counterparts.
Ref:	=2002MNRAS.332..473C
by	COE M.J. , HAIGH N.J., LAYCOCK S.G.T., NEGUERUELA I., KAISER C.R.
	Mon. Not. R. Astron. Soc., 332, 473-478 (2002)
	Observations of the unusual counterpart to the X-ray pulsar AX J0051-733.
o	Table 1: No. 512 = [CSM97] J0050.8-7316 1.
o	Table 1: <[CHL2002] NNN> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHL2004]
[CHL2004]	(Campbell+Harvey+Lester+, 2004)= (SMM) (Not yet in Simbad)
Write:	<<[CHL2004] SMM N>>
N:	6
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	N=6 SMM sources in [WC89] 034.26+0.15 HII core, first designated in Hunter Thesis, 1997.
Ref:	=2004ApJ...600..254C
by	CAMPBELL M.F. , HARVEY P.M., LESTER D.F., CLARK D.M.
	Astrophys. J., 600, 254-268 (2004)
	High-resolution far-infrared observations and models of the star formation core of G34.3+0.2C.
o	In the introd. G34.34+0.13MM is a misprint for G34.24+0.13MM = [HNB98] G34.24+0.13MM
o	Fig.1: <[CHL2004] SMM N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHL2009]
[CHL2009]	(Cheung+Healey+Landt+, 2009)
Write:	<<[C2007] JHHMM+DDMM>>
N:	1
Object:	rG (SIMBAD class: RadioG = Radio Galaxy)
Note:	Newly identified X-shaped radio source in VLA FIRST images. HET (9.2m) and 6.5m MMT spectroscopy.
Ref:	=2009ApJS..181..548C
by	CHEUNG C.C. , HEALEY S.E., LANDT H., VERDOES KLEIJN G.A., JORDAN A.
	Astrophys. J., Suppl. Ser., 181, 548-556 (2009)
	FIRST "Winged" and X-shaped radio source candidates. II. New redshifts.
o	Text, Tables 1-2: <[C2007] J1018+2914>.
=E=	Catalogue in electronic form as J/ApJS/181/548
Origin	of the Acronym: S = Created by Simbad, the CDS Database
History	of this Acronym: replaced by [C2007]
Details on Acronym: CHLT
CHLT	(Choi+Hamaguchi+Lee+Tatematsu)
Write:	<<CHLT NN>>
N:	16
Object:	(cm) (SIMBAD class: cmRad = Centimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 3.5 and 6.2cm continuum observations of the R CrA region.
in source:	NAME R CrA Cloud
Ref:	=2008ApJ...687..406C
by	CHOI M. , HAMAGUCHI K., LEE J.-E., TATEMATSU K.
	Astrophys. J., 687, 406-424 (2008)
	Centimeter imaging of the R Coronae Australis region.
o	Table 2: <CHLT NN> (Nos 1-16).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CHM2006]
[CHM2006]	(CHaty+Hatano+Matsuoka+, 2006)
Write:	<<[CHM2006] Candidate Na>>
N:	6
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	1.4m IRSF at South African Astronomical Observatory, NTT SuSI2, and NTT SofI observations of the field of IGR J17497-2821 to search for candidate counterparts.
Ref:	=2006ATel..906....1C
by	CHATY S. , HATANO H., MATSUOKA Y., NAGATA T.
	ATel, 906, 1 (2006)
	Infrared observations of IGR J17497-2821: new position, new candidate counterparts.
o	<[CHM2006] Candidate N> (Nos 1-6).
Ref:	=2007ApJ...657L.109P
by	PAIZIS A. , NOWAK M.A., CHATY S., RODRIGUEZ J., COURVOISIER T.J.-L., DEL SANTO M., EBISAWA K., FARINELLI R., UBERTINI P., WILMS J.
	Astrophys. J., 657L, 109-112 (2007)
	Unveiling the nature of IGR J17497-2821 using X-ray and near-infrared observations.
o	Fig.2, Table 2: <[CHM2006] Candidate Na> (Nos 1a-1b) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHM2007]
[CHM2007]	(Crook+Huchra+Martimbeau+, 2007)
Write:	<<[CHM2007] LDC NNNN>> <<[CHM2007] HDC NNNN>> <<[CHM2007] LDC NNNN JHHMMSS.ss+DDMMSSs>> <<[CHM2007] HDC NNNN JHHMMSS.ss+DDMMSSs>>
N:	1604+1261+11238+6729
Object:	Group of G + G in Group of G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Search of Group of galaxies and members in the 2MASS redshift survey.
Ref:	=2007ApJ...655..790C
by	CROOK A.C. , HUCHRA J.P., MARTIMBEAU N., MASTERS K.L., JARRETT T., MACRI L.M.
	Astrophys. J., 655, 790-813 (2007)
	Groups of galaxies in the Two Micron All Sky redshift Survey.
o	(Erratum) erratum vol. 685, p. 1320 (2008)
o	Table 6: SimGal = simulated galaxies, formats removed.
o	Table 6: <[CHM2007] LDC NNNN> (Nos 1-1604). Table 7: <[CHM2007] HDC NNNN> (Nos 1-1261). Table 10: <[CHM2007] LDC NNNN JHHMMSS.ss+DDMMSSs> N=11238. Table 11: <[CHM2007] HDC NNNN JHHMMSS.ss+DDMMSSs> N=6729.
=E=	Catalogue in electronic form as J/ApJ/655/790
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHM2009]
[CHM2009]	(CALDWELL+HARDING+MORRISON+2009)
Write:	<<[CHM2009] PHFN-N>> <<[CHM2009] WH2>> <<[CHM2009] JHHMMSSs+DDMMSS>> <<[CHM2009] AHHMMSSs+DDMMSS>> (not recognised by Simbad, but found in literature)
N:	7+1+2
Object:	Poss. GlCl + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Search for star clusters in M31. MMT Hectospec observations. Use of archival HST ACS and WFPC2 data.
in source:	M 31 = NGC 224
Ref:	=2009AJ....137...94C
by	CALDWELL N. , HARDING P., MORRISON H., ROSE J.A., SCHIAVON R., KRIESSLER J.
	Astron. J., 137, 94-110 (2009)
	Star clusters in M31. I. A catalog and a study of the young clusters.
o	Names M088 and M089 inverted in table 1.
o	Tables 1-4: <[CHM2009] PHFN-N> (Nos 4-1, 4-2, 6-1, 6-2, 7-1, 7-2, 8-1). Tables 1-2: <[CHM2009] WH2> N=1. Table 5: <[CHM2009] JHHMMSSs+DDMMSS> N=2.
=E=	Catalogue in electronic form as J/AJ/137/94
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHM2010]
[CHM2010]	(Cannon+ Haynes+Most+, 2010)
Write:	<<[CHM2010] NN>>
N:	18
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	KPNO 0.9m optical observations of the Orion Dwarf Galaxy.
in source:	NAME Orion Dwarf Galaxy
Ref:	=2010AJ....139.2170C
by	CANNON J.M. , HAYNES K., MOST H., SALZER J.J., HAUGLAND K., SCUDDER J., SUGDEN A., WEINDLING J.
	Astron. J., 139, 2170-2183 (2010)
	The stellar and gaseous contents of the Orion dwarf galaxy.
o	Table 2: <[CHM2010] NN> (Nos 1-18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHM2018]
[CHM2018]	(Cai+Hamden+Matuszewski+, 2018) (Not yet in Simbad)
Write:	<<[CHM2018] ELAN0101+0201>> <<[CHM2018] ELAN0101+0201 QN>> <<[CHM2018] ELAN0101+0201 LAEN>>
N:	1+2+4
Object:	Lyman Alpha Nebula + QSO + Poss. LAE (SIMBAD class: EmObj = Emission Object)
Note:	Keck and Palomar Cosmic Web Imagers (KCWI/PCWI) observations of N=1 Enormous Lyman α nebula (ELAN), associated with N=2 QSO and N=4 Lyman α emitters (LAEs) candidates.
Ref:	=2018ApJ...861L...3C
by	CAI Z. , HAMDEN E., MATUSZEWSKI M., PROCHASKA J.X., LI Q., CANTALUPO S., ARRIGONI BATTAIA F., MARTIN C., NEILL J.D., O'SULLIVAN D., WANG R., MOORE A., MORRISSEY P.
	Astrophys. J., 861L, 3-3 (2018)
	Keck/Palomar Cosmic Web Imagers reveal an enormous Lyα nebula in an extremely overdense quasi-stellar object pair field at z = 2.45.
o	Figs 2-3, Table 1: <[CHM2018] ELAN0101+0201> N=1, <[CHM2018] ELAN0101+0201 QN> (Nos Q1 to Q2), <[CHM2018] ELAN0101+0201 LAEN> (Nos LAE1 to LAE4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHM98]
[CHM98]	(Cappi+Held+Marano, 1998)
Write:	<<[CHM98] Cl 0053-37 NN>> <<[CHM98] Cl 0053-37 A>> <<[CHM98] ACO 3889 NN>> <<[CHM98] ACO 3889 FN>> <<[CHM98] ACO 3663 N>> <<[CHM98] ACO 3663 A>>
N:	22+26+6
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table 2: (Nos 1-21), galaxies in ClG 0053-37, No. B is a Background galaxy Table 3: (Nos 1-24), galaxies in ACO 3889 (Nos F1-F2) are Foreground galaxies Table 4: (Nos 1-5), galaxies in ACO 3663 No. B is a Background galaxy
in source:	ClG 0053-37
in source:	ACO 3889
in source:	ACO 3663
Ref:	=1998A&AS..129...31C
by	CAPPI A. , HELD E.V., MARANO B.
	Astron. Astrophys., Suppl. Ser., 129, 31-40 (1998)
	Galaxy redshifts in 3 medium-distant clusters.
o	Table 2: <[CHM98] Cl 0053-37 NN> (Nos 1-21), <[CHM98] Cl 0053-37 B>. Table 3: <[CHM98] ACO 3889 NN> (Nos 1-24), <[CHM98] ACO 3889 FN> (Nos F1-F2). Table 4: <[CHM98] ACO 3663 N> (Nos 1-5), <[CHM98] ACO 3663 B>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ChMM
ChMM	(Choi, millimeter)
Write:	<<ChMM N>>
N:	2
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=2 mm sources in HH 170-110 region. See also ChCl.
in source:	NAME HH 270-110
Ref:	=2001ApJ...550..817C
by	CHOI M.
	Astrophys. J., 550, 817-823 (2001)
	Observations of molecular clouds in the HH 270/110 region.
o	Table 1, Fig.1: <ChMM N> (Nos 1-2). Fig.4: <ChCl A> (Nos A-B).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CHN2017]
[CHN2017]	(Chibueze+Hamabata+Nagayama+, 2017)
Write:	<<[CHN2017] Sh2-76EMMN>> <<[CHN2017] Sh2-76EMMN NN>>
N:	2+36
Object:	YSO + Maser (SIMBAD class: YSO = Young Stellar Object)
Note:	VERA VLBI H2O maser observations of N=26+10 masers associated with N=2 YSOs in the Sharpless-76E star forming region.
in source:	SH 2-76 E
Ref:	=2017MNRAS.466.4530C
by	CHIBUEZE J.O. , HAMABATA H., NAGAYAMA T., OMODAKA T., HANDA T., SUNADA K., NAKANO M., UENO Y.
	Mon. Not. R. Astron. Soc., 466, 4530-4534 (2017)
	Sharpless-76E: astrometry and outflows in a protostellar cluster.
o	Table 2: <[CHN2017] Sh2-76EMMN> (Nos EMM1-EMM2). Table 3: <[CHN2017] Sh2-76EMM1 NN> (Nos 1-26). Table 4: <[CHN2017] Sh2-76EMM2 NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHO2012]
[CHO2012]	(Cheung+Hays+Ojha+, 2012)
Write:	<<[CHO2012] XRTN>>
N:	4
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Swift observations of N=4 X-ray sources, in the search for potential counterparts to the gamma-ray transient source Fermi J0902-4624.
Ref:	=2012ATel.3973....1C
by	CHEUNG C.C. , HAYS E., OJHA R., DONATO D., KENNEA J.A.
	ATel, 3973, 1 (2012)
	Swift/XRT Follow-up of the Fermi-LAT Galactic Plane Transient J0902-4624.
o	<[CHO2012] XRTN> (Nos XRT1-XRT4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ChOPS
ChOPS	(Champlane Optical Plane Survey)
Write:	<<ChOPS JHHMMSS.ss+DDMMSS.s>>
N:	10000000
Object:	* (SIMBAD class: Star)
Note:	Catalog of optical sources in the ChaMPlane multiwavelength survey. 2006ApJS..163..160R: 1st ref. with ChOPS and CXOPS objects.
Notes:	ChaMPlane is a multiwavelength survey. This catalog (ChOPS) of optical sources will be joined by an X-ray catalog CXOPS. The two catalogs reference each other to provide X-ray and optical data, flux ratios etc for sources detected in both our Chandra and NOAO surveys. Infrared data will also be obtained and will follow the same convention, a separate IR catalog will be released ChIPS with cross-referencing to the 2 others.
Notes:	The Chandra Multiwavength Plane (ChaMPlane) Survey of the galactic plane incorporates serendipitous sources from selected Chandra pointings in or near the galactic plane (b < 12deg, >20 ksec, lack of bright diffuse or point sources) to measure or constrain the luminosity function of low-luminosity accretion sources in the Galaxy. The primary goal is to detect and identify accreting white dwarfs (cataclysmic variables, with space density still uncertain by a factor of >10-100), neutron stars and black holes (quiescent low mass X-ray binaries) to constrain their space densities and thus origin and evolution. Secondary objectives are to identify Be stars in high mass X-ray binaries and constrain their space densities, and to survey the H-R diagram for stellar coronal sources. A parallel optical imaging under the NOAO Long Term Survey program provides deep optical images using the Mosaic imager on the CTIO and KPNO 4-m telescopes. The 36x36arcmin optical images (Halpha, R, V and I) cover 5X the area of each enclosed Chandra ACIS FOV, providing an extended survey of emission line objects for comparison with Chandra. Spectroscopic followup of optical counterparts is then conducted, thus far with WIYN and Magellan. This catalog contains all ChaMPlane optical point sources, their positions, V,R,I,Halpha magnitudes and links to probable counterparts in our X-ray catalog. The reduced images are available through NOAO. http://hea-www.harvard.edu/ChaMPlane
Ref:	=2006ApJS..163..160R
by	ROGEL A.B. , LUGGER P.M., COHN H.N., SLAVIN S.D., GRINDLAY J.E., ZHAO P., HONG J.
	Astrophys. J., Suppl. Ser., 163, 160-172 (2006)
	Three years of ChaMPlane northern field WIYN spectroscopy.
o	Tables 4 to 8: <ChOPS JHHMMSS.ss+DDMMSS.s> N=5+4+7+2+4. Tables 6 to 8: <CXOPS JHHMMSS.s+DDMMSS> N=7+5+26. Table 4: <[RLC2006] CVN> (Nos CV1-CV5), <[RLC2006] XBN> (Nos XB1, XB2).
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [CHP2004]
[CHP2004]	(Colbert+Heckman+Ptak+, 2004)
Write:	<<[CHP2004] JHHMMSS.s+DDMMSS>>
N:	1441
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS observations of 32 galaxies.
Ref:	=2004ApJ...602..231C
by	COLBERT E.J.M. , HECKMAN T.M., PTAK A.F., STRICKLAND D.K., WEAVER K.A.
	Astrophys. J., 602, 231-248 (2004)
	Old and young X-ray point source populations in nearby galaxies.
o	Table A1: <[CHP2004] JHHMMSS.s+DDMMSS> N=1441.
=E=	Catalogue in electronic form as J/ApJ/602/231
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CHR
CHR	(Center for High Resolution)= (CHA) = (CHARA)
Write:	<< CHR NNNAA>> << CHR NNNAa>>
Object:	(SIMBAD class: = Double or Multiple Star)
Origin	of the Acronym: L (1996AJ....112.2260M)
Details on Acronym: [CHR2013]
[CHR2013]	(Clowes+Harris+Raghunathan+, 2013)
Write:	<<[CHR2013] U1.27>>
N:	1
Object:	Large Quasar Group (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=1 large quasar group found in the DR7QSO catalogue of the SDSS. In the format, the letter U refers to a connected unit of quasars, and the number refers to the mean redshift. See also [CCG2012].
Ref:	=2013MNRAS.429.2910C
by	CLOWES R.G. , HARRIS K.A., RAGHUNATHAN S., CAMPUSANO L.E., SOCHTING I.K., GRAHAM M.J.
	Mon. Not. R. Astron. Soc., 429, 2910-2916 (2013)
	A structure in the early universe at z ~ 1.3 that exceeds the homogeneity scale of the R-W concordance cosmology.
o	<[CHR2013] U1.27> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CHS
CHS	(Carpenter+Hillebrand+Skrutskie)
*****	Avoid the usage of CHS, prefer [CHS2001]
Origin	of the Acronym: L (2002ApJ...574..258F)
Details on Acronym: [CHS2001]
[CHS2001]	(Carpenter+Hillebrand+Skrutskie, 2001)= (CHS)
Write:	<<[CHS2001] NNNNN>>
N:	1235
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	NIR photometry of 18552 stars toward Ori A MCld, from 2MASS telescope, not part of the first and second incremental release catalogues. Among them, 1235 are V*.
in source:	NAME Ori A
Ref:	=2001AJ....121.3160C
by	CARPENTER J.M. , HILLENBRAND L.A., SKRUTSKIE M.F.
	Astron. J., 121, 3160-3190 (2001)
	Near-infrared photometric variability of stars toward the Orion A molecular cloud.
o	Table 4: <[CHS2001] NNNNN> N=1235 among 18552.
=E=	Catalogue in electronic form as J/AJ/121/3160
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHS2005]
[CHS2005]	(Coppin+Halpern+Scott+, 2005)= (GSS)
Write:	<<[CHS2005] GSS 850.NN>>
N:	11
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	850mu.m map and list of candidate sources in a subarea of the Groth Strip observed using SCUBA.
in source:	NAME Groth-Westphal Strip
Ref:	=2005MNRAS.357.1022C
by	COPPIN K. , HALPERN M., SCOTT D., BORYS C., CHAPMAN S.
	Mon. Not. R. Astron. Soc., 357, 1022-1028 (2005)
	An 850-µm SCUBA map of the Groth Strip and reliable source extraction.
o	Fig.1, Tables 1, 2: <[CHS2005] GSS 850.NN> (Nos .1 to .11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHS2007]
[CHS2007]	(Cheung+Harris+Stawarz, 2007) (Not yet in Simbad)
Write:	<<[CHS2007] HST-1 aN>>
N:	4+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	NRAO VLBA observations of [PBZ99] HST-1.
in source:	M 87:[PBZ99] HST-1 = [PBZ99] HST-1
Ref:	=2007ApJ...663L..65C
by	CHEUNG C.C. , HARRIS D.E., STAWARZ L.
	Astrophys. J., 663L, 65-68 (2007)
	Superluminal radio features in the M87 jet and the site of flaring TeV γ-ray emission.
o	Figs 1,4: <[CHS2007] HST-1 aN> (Nos a-d, c1-c2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CHS95]
[CHS95]	(Cowie+Hu+Songaila, 1995) (Not yet in Simbad)
Write:	<<[CHS95] NN-NN>>
N:	211
Object:	* + G (SIMBAD class: Star)
Note:	HST WFPC2 Plates 83-91: Atlas of objects in the HST WFC fields SSA 13 and 22: (SSA fields are defined in 1991ApJ...369...79L) In the format 'NN-NN' the left 'NN' stands for the Figure no., Figs 10 to 15 and 18 to 20: Fig. 10, Plate 83: format '10-NN', (Nos 0-21) Fig. 11, Plate 84: format '11-NN', (Nos 0-16) Fig. 12, Plate 85: format '12-NN', (Nos 0-21) Fig. 13, Plate 86: format '13-NN', (Nos 0-24) Fig. 14, Plate 87: format '14-NN', (Nos 0-19) Fig. 15, Plate 88: format '15-NN', (Nos 0-12) Fig. 18, Plate 89: format '18-NN', (Nos 0-26) Fig. 19, Plate 90: format '19-NN', (Nos 0-41) Fig. 20, Plate 91, and Table 1: chain galaxies, format '20-NN', (Nos 0-27)
Ref:	=1995AJ....110.1576C
by	COWIE L.L. , HU E.M., SONGAILA A.
	Astron. J., 110, 1576-1583 (1995)
	Faintest galaxy morphologies from HST WFPC2 imaging of the Hawaii survey fields.
o	p. 1582: SSA 22-16 and 24 = LCG SSA 22-16 and 24
o	Figs 10-15, 18-20: <[CHS95] NN-NN> N=211
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CHSM
CHSM	(Carpenter+Hillebrand+Skrutskie+Meyer)
Write:	<<CHSM NNNNN>>
N:	95+5+
Object:	* (SIMBAD class: Star)
Note:	NIR photometry of 34354 stars toward Cha I, from 2MASS telescope. Among the stars, 95 are V*.
in source:	NAME Cha I
Ref:	=2002AJ....124.1001C
by	CARPENTER J.M. , HILLENBRAND L.A., SKRUTSKIE M.F., MEYER M.R.
	Astron. J., 124, 1001-1025 (2002)
	Near-infrared photometric variability of stars toward the Chamaeleon I molecular cloud.
o	Tables 3, 4, 6: <CHSM NNNNN> N = 95+5+ among 34354.
=E=	Catalogue in electronic form as J/AJ/124/1001
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CHSS
CHSS	(Century Halo Star Survey)
Write:	<<CHSS NNNN>>
N:	4015
Object:	* (SIMBAD class: Star)
Note:	The Century Halo Star Survey (CHSS) is a photometric and spectroscopic survey from which the authors select relatively blue stars as probes of the Milky Way halo. Additional data from 2MASS is also used. Spectral follow-up with Whipple Observatory 1.5m telescope.
Ref:	=2003AJ....126.1362B
by	BROWN W.R. , ALLENDE PRIETO C., BEERS T.C., WILHELM R., GELLER M.J., KENYON S.J., KURTZ M.J.
	Astron. J., 126, 1362-1380 (2003)
	The Century Survey Galactic Halo project. I. Stellar spectral analysis.
o	Table 7: <CHSS NNN> N=764 among (Nos 1-901).
Ref:	=2005AJ....130.1097B
by	BROWN W.R. , GELLER M.J., KENYON S.J., KURTZ M.J., ALLENDE PRIETO C., BEERS T.C., WILHELM R.
	Astron. J., 130, 1097-1110 (2005)
	The Century Survey Galactic Halo Project. II. Global properties and the luminosity function of field blue horizontal branch stars.
o	Tables 2, 3: <CHSS NNNN> (Nos 902-1689) added.
Ref:	=2008AJ....135..564B
by	BROWN W.R. , BEERS T.C., WILHELM R., ALLENDE PRIETO C., GELLER M.J., KENYON S.J., KURTZ M.J.
	Astron. J., 135, 564-574 (2008)
	The Century Survey Galactic Halo Project. III. A complete 4300°^{2} survey of blue horizontal branch stars in the metal-weak thick disk and inner halo.
o	Table 2: <CHSS NNNN> (Nos 1690-4015) added.
=E=	Catalogue in electronic form as J/AJ/126/1362
=E=	Catalogue in electronic form as J/AJ/130/1097
=E=	Catalogue in electronic form as J/AJ/135/564
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CHT80]
[CHT80]	(Campbell+Hoffmann+Thronson+, 1980)= (FIR)
Write:	<<[CHT80] FIR NN>>
N:	49
Object:	(Far IR) (SIMBAD class: FarIR = Far-IR source (λ >= 30 µm))
Note:	Far IR survey made with a ballon-borne 40cm telescope.
in source:	NAME Cyg X
Ref:	=1980ApJ...238..122C
by	CAMPBELL M.F. , HOFFMANN W.F., THRONSON H.A., HARVEY P.M.
	Astrophys. J., 238, 122-132 (1980)
	Far-infrared survey of Cygnus X.
o	Table 1: <[CHT80] FIR NN> (Nos 1-49).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Chupina
Chupina	(Chupina)
Write:	<<Cl Chupina N>>
N:	5
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Note:	Found in 2010A&A...516A...3K.
=E=	Catalogue in electronic form as B/ocl
Origin	of the Acronym: L (2010A&A...516A...3K)
Details on Acronym: CHVC
CHVC	(Compact High-Velocity Cloud)
*****	Avoid the usage of CHVC, prefer HVC
Origin	of the Acronym: L (2001A&A...369..616B)
Details on Acronym: CHX
CHX	(Chamaeleon, X-ray source)
Write:	<<CHX NNW>> <<CHX NNa>>
N:	22+19
Object:	(Soft X) (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	1st ref.: Table 2: (Nos 1-22) IPC X-ray sources Table 4: N=15 optical candidates, format 'NNa' to differentiate them with the X-ray sources format 'NN'. 2nd ref.: The authors introduce a format 'NNW' for X-ray sources. See also Wa, CrAPMS, ScoPMS
Ref:	=1989ApJ...338..262F
by	FEIGELSON E.D. , KRISS G.A.
	Astrophys. J., 338, 262-276 (1989)
	Soft X-ray observations of pre-main-sequence stars in the Chamaeleon dark cloud.
o	Table 2: <CHX NN> N=22, Table 4: <CHX NNa> N=15
Ref:	=1992AJ....104..758W
by	WALTER F.M.
	Astron. J., 104, 758-761 (1992)
	X-ray sources in regions of star formation. IV. High-resolution optical spectroscopy of X-ray identified candidate pe-main-sequence stars in the Chamaeleon I Cloud.
o	<CHX NNW> (Nos 18N, 18S, 20E)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CHXR
CHXR	(Chamaeleon, X-ray source, ROSAT satellite)
Write:	<<CHXR NNA>> <<CHXR NNWW>>
N:	89+19
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT observations of cha I cloud. 1st ref., Tables 2,3: (Nos 1-89). Identif. charts. 2nd and 3rd ref.: formats 'NNA', 'NNW' and 'NNWW' are added. See also CHIIXR.
in source:	NAME Cha I
Ref:	=1993ApJ...416..623F
by	FEIGELSON E.D. , CASANOVA S., MONTMERLE T., GUIBERT J.
	Astrophys. J., 416, 623-646 (1993)
	ROSAT X-ray study of the Chamaeleon I dark cloud. I. The stellar population.
o	Table 4, col. 7: ASS CHA T 2-NNa, Table 6 : GK-1 = HBC 582
o	<CHXR NN> (Nos 1-89)
Ref:	=1994MNRAS.271..967H
by	HUENEMOERDER D.P. , LAWSON W.A., FEIGELSON E.D.
	Mon. Not. R. Astron. Soc., 271, 967-975 (1994)
	X-ray-selected T Tauri stars in the Chamaeleon I cloud.
o	CHXR 68p = CHXR 68A
o	Table 1: <CHXR NNA>, <CHXR NNWW> N=5 new obj.
Ref:	=1996MNRAS.280.1071L
by	LAWSON W.A. , FEIGELSON E.D., HUENEMOERDER D.P.
	Mon. Not. R. Astron. Soc., 280, 1071-1088 (1996)
	An improved HR diagram for Chamaeleon I pre-main-sequence stars.
o	GK-1 = HBC 582
o	Tables 1, 2: <CHXR NNA>, <CHXR NNWW> N=13 new obj. Table 1: <CHX NNW> N=2 new obj.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CHXX
CHXX	(Chamaeleon, X-ray source, XMM-Newton)
Write:	<<CHXX NN>>
N:	71
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of Cha I dark cloud.
in source:	NAME Cha I
Ref:	=2007A&A...461..669R
by	ROBRADE J. , SCHMITT J.H.M.M.
	Astron. Astrophys., 461, 669-678 (2007)
	A deep XMM-Newton X-ray observation of the Chamaeleon I dark cloud.
o	Table 4: The first number 71 is a misprint for 70!
o	Table 4: <CHXX NN> (Nos 1-71).
=E=	Catalogue in electronic form as J/A+A/461/669
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CHY91]
[CHY91]	(Condon+Huang+Yin+, 1991)
Write:	<<[CHY91] HHMMSS.ss+DDMMSS.s>> <<[CHY91] HHMMSS.s+DDMMSS>>
N:	51
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	N=51 radio components of 39 galaxies.
Ref:	=1991ApJ...378...65C
by	CONDON J.J. , HUANG Z.-P., YIN Q.F., THUAN T.X.
	Astrophys. J., 378, 65-76 (1991)
	Compact starbursts in ultraluminous infrared galaxies.
o	Table 2: <[CHY91] HHMMSS.ss+DDMMSS.s>, <[CHY91] HHMMSS.s+DDMMSS>, N=51.
=E=	Catalogue in electronic form as J/ApJ/378/65
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ci
Ci	(Cincinnati Publ.)= (C) = Cin
Write:	<<Ci 18 NNNN>> <<Ci 20 NNNN>>
N:	3164+1474
Object:	PM* (SIMBAD class: HighPM* = High Proper Motion Star)
Note:	In the format, '18' or '20' stand for Cincinnati Publ. 18 and 20
Ref:	=1918PCinO..18d...1P
by	PORTER J.G. , YOWELL E.J., SMITH E.S.
	Publ. Cincinnati Obs., 18, part no 4, 1-57 (1918)
	Catalogue of proper motion stars .
o	Catalogue: <Ci 18 NNNN> (Nos 1-3164)
Ref:	=1930PCinO..20....1P
by	PORTER J.G. , YOWELL E.J., SMITH E.S.
	Publ. Cincinnati Obs., 20, 1-None (1930)
	A catalogue of 1474 stars with proper motion exceeding .4"/year.
o	Catalogue: <Ci 20 NNNN> (Nos 1-1474)
Details on Acronym: [CI95]
[CI95]	(Chevalier+Ilovaisky, 1995)
Write:	<<[CI95] NN>>
N:	9
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	OHP 1.2m telescope observations. Comparison stars in the field of GRO J0422+32. See also [BSN97].
Ref:	=1995A&A...297..103C
by	CHEVALIER C. , ILOVAISKY S.A.
	Astron. Astrophys., 297, 103-114 (1995)
	CCD photometry of GRO J0422+32 during activity and quiescence.
o	Fig.1, Table 1: <[CI95] NN> (Nos 2-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CIA91]
[CIA91]	(Corrigan+Irwin+Arnaud+, 1991)
Write:	<<[CIA91] ggg>>
N:	2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=2 stars 'alf' and 'bet' in the field of QSO 2237+0305 Map in Fig. 1
Ref:	=1991AJ....102...34C
by	CORRIGAN R.T. , IRWIN M.J., ARNAUD J., FAHLMAN G.G., et al.
	Astron. J., 102, 34-40 (1991)
	Initial light curve of Q2237+0305.
o	Components A to D of Q2237+0305 = [Y88] A to [Y88] D
o	Table 2: <[CIA91] alf>, <[CIA91] bet>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CID
CID	(Cluster ID number)
Write:	<<CID NN>>
N:	85
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table 1, col.(1): N=84 ClG (Nos 1-84) + No. 90 No. 90 = Coma cluster, primary reference cluster. all CID are cross-id. with ACO or [WCB96] in the last col. See also the G in ClG GIN NNN in Table 3, and ClG numbering CAN in Paper II.
Ref:	=1996ApJS..106....1W
by	WEGNER G. , COLLESS M., BAGGLEY G., DAVIES R.L., BERTSCHINGER E., BURSTEIN D., McMAHAN R.K.Jr, SAGLIA R.P.
	Astrophys. J., Suppl. Ser., 106, 1-26 (1996)
	The peculiar motions of early-type galaxies in two distant regions. I. Cluster and galaxy selection.
o	Table 1: <CID NN> (Nos 1-84, 90), with N=49 cross-id. in last col.: <[WCB96] ACO NNN-N>, <[WCB96] ACO NNNN-W>, <[WCB96] JNN>, <[WCB96] JNN-N>, <[WCB96] JNNW>, <[WCB96] PNNN-N>. Table 3: <GIN NNN> (Nos 1-801), with N=749 cross-id. in col.(2): <[WCB96] ACO NNNN A>, <[WCB96] ACO NNNN N>, <[WCB96] ACO NNN-N A>, <[WCB96] ACO NNN-N N>, <[WCB96] ACO NNNN-W A>, <[WCB96] ACO NNNN-W N>, <[WCB96] JNN A>, <[WCB96] JNN N>, <[WCB96] JNN/NN N>, <[WCB96] JNN-N A>, <[WCB96] JNN-N N>, <[WCB96] JNNW A>, <[WCB96] JNNW N>, <[WCB96] PNNN-N A>, <[WCB96] PNNN-N N>
=E=	Catalogue in electronic form as J/ApJS/106/1
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CID
CID	(Chandra ID)
*****	Avoid the usage of CID, prefer [ECV2009]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CID2000]
[CID2000]	(Coziol+Iovino+De Carvalho, 2000)
Write:	<<[CID2000] HHMM+DDMM>> <<[CID2000] HHMM+DDMM A>> <<[CID2000] HHMM+DDMM Ac>>
N:	49+193
Object:	Group of G + G in Group (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=49 southern compact groups, format 'HHMM+DDMM'. N=193 galaxies in the groups, , format 'HHMM+DDMM A', and format 'HHMM+DDMM Ac', this format indicates that the galaxies 'A' and 'Ac' seen to be in a merger phase.
Ref:	=2000AJ....120...47C
by	COZIOL R. , IOVINO A., DE CARVALHO R.R.
	Astron. J., 120, 47-67 (2000)
	The relation between activity and environment in compact groups of galaxies.
o	Table 1: <[CID2000] HHMM+DDMM> N=49. Table 1: <[CID2000] HHMM+DDMM A>, <[CID2000] HHMM+DDMM Ac>, N=193.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CIDA
CIDA	(Centro de Investigacines De Astronomia)
*****	Avoid the usage of CIDA, prefer [BCG93]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CIF2003]
[CIF2003]	(Carilli+Ivison+Frail, 2003)
Write:	<<[CIF2003] JHHMMSS.ss+DDMMSS.s>>
N:	8
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 1.4GHz observations of the Lockman Hole region.
in source:	NAME Lockman Hole
Ref:	=2003ApJ...590..192C
by	CARILLI C.L. , IVISON R.J., FRAIL D.A.
	Astrophys. J., 590, 192-196 (2003)
	Variability of submillijansky radio sources.
o	Tables 2, 3: <[CIF2003] JHHMMSS.ss+DDMMSS.s> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CIF2008]
[CIF2008]	(Cioni+Irwin+Ferguson+, 2008)
Write:	<<[CIF2008] DD.dddddd+DD.dddddd>>
N:	7650
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	UKIRT WFCAM NIR observations of M33.
in source:	M 33 = NGC 598
Ref:	=2008A&A...487..131C
by	CIONI M.-R.L. , IRWIN M., FERGUSON A.M.N., McCONNACHIE A., CONN B.C., HUXOR A., IBATA R., LEWIS G., TANVIR N.
	Astron. Astrophys., 487, 131-146 (2008)
	AGB stars as tracers of metallicity and mean age across M33.
o	(Erratum) erratum vol. 500, p. 1025 (2009)
o	Table 1: <[CIF2008] DD.dddddd+DD.dddddd> N=7650.
=E=	Catalogue in electronic form as J/A+A/487/131
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CIG
CIG	(Catalog of Isolated G)
*****	Avoid the usage of CIG, prefer K73
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [CII2008]
[CII2008]	(Chapman+Ibata+Irwin+, 2008)
Write:	<<[CII2008] JHHMMSS.ss+DDMMSS.s>>
N:	18+17+35+30+12+4
Object:	Star (SIMBAD class: Star)
Note:	Keck II DEIMOS observations of Andromeda's halo.
Ref:	=2008MNRAS.390.1437C
by	CHAPMAN S.C. , IBATA R., IRWIN M., KOCH A., LETARTE B., MARTIN N., COLLINS M., LEWIS G.F., McCONNACHIE A., PENARRUBIA J., RICH R.M., TRETHEWEY D., FERGUSON A., HUXOR A., TANVIR N.
	Mon. Not. R. Astron. Soc., 390, 1437-1452 (2008)
	The kinematic footprints of five stellar streams in Andromeda's halo.
o	Tables 2-5: <[CII2008] JHHMMSS.ss+DDMMSS.s> N=18+17+35+29. Tables 6-7: <[CII2008] JHHMMSS.s+DDMMSS.s> N=12+4. Text, Table 1: <NAME M31 Stream Ca> (Nos Cr-Cp).
=E=	Catalogue in electronic form as <J/MNRAS/390/1437/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CIII
CIII	(Constellation III (roman num.))
Write:	<<CIII {X\|Y\|Z}NNN>>
N:	40 among 956
Object:	Red * (SIMBAD class: Star)
Note:	Table 2: Red stars in 3 fields 'X, Y, Z'.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1987ApJ...321..156M
by	MOULD J. , REID N.
	Astrophys. J., 321, 156-161 (1987)
	The evolution of asymptotic giant branch stars in the Magellanic Clouds. III. The problem of intermediate-mass stars.
o	Table 1: <BLMC NN> N=20 among (Nos 1-55), Table 2: <CIII XNNN>, <CIII YNNN> and <CIII ZNNN> N=35
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CIL2015]
[CIL2015]	(Caputi+Ilbert+Laigle+, 2015)
Write:	<<[CIL2015] NNNNNN>>
N:	9
Object:	Poss. G (SIMBAD class: Galaxy_Candidate = Galaxy Candidate)
Note:	Identification of N=9 galaxy candidates at z≥5 in the UltraVISTA ultradeep COSMOS field. Use of archival Spitzer IRAC data.
in source:	NAME COSMOS Field
Ref:	=2015ApJ...810...73C
by	CAPUTI K.I. , ILBERT O., LAIGLE C., McCRACKEN H.J., LE FEVRE O., FYNBO J., MILVANG-JENSEN B., CAPAK P., SALVATO M., TANIGUCHI Y.
	Astrophys. J., 810, 73 (2015)
	Spitzer bright, UltraVISTA faint sources in COSMOS: the contribution to the overall population of massive galaxies at z = 3-7.
o	Table 3: <[CIL2015] NNNNNN> N=9 among (Nos 66110-260169).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CIL99]
[CIL99]	(Chevalier+Ilovaiski+Leisy+, 1999)
Write:	<<[CIL99] Star a>> <<[CIL99] CN>>
N:	5+2
Object:	* (SIMBAD class: Star)
Note:	Search for the optical counterpart of Aql X-1: N=5 stars in the field. The true counterpart is 'Star e', the interloper star from 1999IAUC.7086S...1C. N=2 comparison stars (Nos C1-C2).
in source:	X Aql X-1
Ref:	=1999A&A...347L..51C
by	CHEVALIER C. , ILOVAISKY S.A., LEISY P., PATAT F.
	Astron. Astrophys., 347, 51-54 (1999)
	Magnitude, color and spectral type of Aql X-1 in quiescence.
o	Table 1: <[CIL99] Star a> (Nos a-e). Text: <[CIL99] CN> (Nos C1-C2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CIM2002]
[CIM2002]	(Calchi Novati+Iovane+Marino+, 2002)
Write:	<<[CIM2002] N>>
N:	6
Object:	Poss. Microlensing Event (SIMBAD class: LensingEv = (Micro)Lensing Event)
Stat:	is completely incorporated in Simbad
Note:	First results of a search for microlensing events in M 31. See also [CJS2003].
in source:	M 31 = NGC 224
Ref:	=2002A&A...381..848C
by	CALCHI NOVATI S. , IOVANE G., MARINO A.A., AURIERE M., BAILLON P., BOUQUET A., BOZZA V., CAPACCIOLI M., CAPOZZIELLO S., CARDONE V., COVONE G., DE PAOLIS F., DE RITIS R., GIRAUD-HERAUD Y., GOULD A., INGROSSO G., JETZER P., KAPLAN J., LAMBIASE G., LE DU Y., MANCINI L., PIEDIPALUMBO E., RE V., RONCADELLI M., RUBANO C., SCARPETTA G., SCUDELLARO P., SERENO M., STRAFELLA F.
	Astron. Astrophys., 381, 848-861 (2002)
	Microlensing search towards M 31.
o	Table 2: <[CIM2002] N> (Nos 1-5).
Ref:	=2003A&A...405..851C
by	CALCHI NOVATI S. , JETZER P., SCARPETTA G., GIRAUD-HERAUD Y., KAPLAN J., PAULIN-HENRIKSSON S., GOULD A.
	Astron. Astrophys., 405, 851-857 (2003)
	Microlensing towards M 31 with MDM data.
o	Table 1: Objects T1 to T5 = [CIM2002] 1 to 5, so T6 is designated as [CIM2002] 6 in SIMBAD.
o	Table 1: <[CIM2002] N> (No. 6) added. Tables 1, 2: <[CJS2003] CN> (Nos C1-C5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Cin
Cin	(Cincinnati Publ.)
====>	Equivalent to: Ci
Details on Acronym: CiPg
CiPg	(Caloi+Panagia) (Not yet in Simbad)
====>	Equivalent to: CaPa
Details on Acronym: Cir
Cir	(Circinus)
*****	Avoid the usage of Cir, prefer [ABC89]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CIR2010]
[CIR2010]	(Chapman+Ivison+Roseboom+, 2010)
Write:	<<[CIR2010] JHHMMSS.sss+DDMMSS.ss>>
N:	20+21
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Herschel SPIRE observations of ultraluminous infrared galaxies.
Ref:	=2010MNRAS.409L..13C
by	CHAPMAN S.C. , IVISON R.J., ROSEBOOM I.G., AULD R., BOCK J., BRISBIN D., BURGARELLA D., CHANIAL P., CLEMENTS D.L., COORAY A., EALES S., FRANCESCHINI A., GIOVANNOLI E., GLENN J., GRIFFIN M., MORTIER A.M.J., OLIVER S.J., OMONT A., PAGE M.J., PAPAGEORGIOU A., PEARSON C.P., PEREZ-FOURNON I., POHLEN M., RAWLINGS J.I., RAYMOND G., RODIGHIERO G., ROWAN-ROBINSON M., SCOTT D., SEYMOUR N., SMITH A.J., SYMEONIDIS M., TUGWELL K.E., VACCARI M., VIEIRA J.D., VIGROUX L., WANG L., WRIGHT G.
	Mon. Not. R. Astron. Soc., 409L, 13-18 (2010)
	Herschel-SPIRE, far-infrared properties of millimetre-bright and -faint radio galaxies.
o	Table S1: <[CIR2010] JHHMMSS.sss+DDMMSS.ss> N=20+21.
=E=	Catalogue in electronic form as J/MNRAS/409/L13
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CIRSI
CIRSI	(Cambridge IR Survey Instrument)
Write:	<<CIRSI NN>>
N:	22
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	INT Wide Angle Survey, Las Campanas IR survey and Infrared CIRSI-INT survey observations. Quasar selection using NIR and optical images.
Ref:	=2002MNRAS.337.1153S
by	SHARP R.G. , SABBEY C.N., VIVAS A.K., OEMLER A.Jr, McMAHON R.G., HODGKIN S.T., COPPI P.S.
	Mon. Not. R. Astron. Soc., 337, 1153-1162 (2002)
	Reddening-independent quasar selection from a wide-field optical and near-infrared imaging survey.
o	p.1155: NGC 0450:0126-0019 = [GMS97] NGC 450 99
o	Table 2: <CIRSI NN> (Nos 1-22).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CIT
CIT	(California Inst. of Technology)
Write:	<<CIT NN>>
N:	14
Object:	Cool * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1966ApJ...146..288U
by	ULRICH B.T. , NEUGEBAUER G., McCAMMON D., LEIGHTON R.B., HUGHES E.E., BECKLIN E.
	Astrophys. J., 146, 288-290 (1966)
	Further observations of extremely cool stars.
o	Table 1: <CIT NN> (Nos 1-14)
Details on Acronym: [CIV2009]
[CIV2009]	(Cedres+Iglesias-Paramo+Vilchez+, 2009)
Write:	<<[CIV2009] SDSS SDSSJ160528.84+174906.2B>>
N:	1
Object:	Halpha emitter (SIMBAD class: Galaxy)
Note:	NOT and WHT Hα observations of the central regions of ACO 2151.
Ref:	=2009AJ....138..873C
by	CEDRES B. , IGLESIAS-PARAMO J., VILCHEZ J.M., REVERTE D., PETROPOULOU V., HERNANDEZ-FERNANDEZ J.
	Astron. J., 138, 873-888 (2009)
	Star-forming galaxies in the Hercules cluster: Hα imaging of A2151.
o	Table 2: <[CIV2009] SDSS SDSSJ160528.84+174906.2B> N=1.
=E=	Catalogue in electronic form as J/AJ/138/873
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CIZA
CIZA	(Cluster In the Zone of Avoidance)
Write:	<<CIZA JHHMM.m+DDMM>>
N:	73+57
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	X-ray brightest clusters from the CIZA survey. Clusters are selected from the RASS.
Ref:	=2002ApJ...580..774E
by	EBELING H. , MULLIS C.R., TULLY R.B.
	Astrophys. J., 580, 774-788 (2002)
	A systematic X-ray search for clusters of galaxies behind the Milky Way.
o	Table 1: <CIZA JHHMM.m+DDMM> N=73.
Ref:	=2007ApJ...662..224K
by	KOCEVSKI D.D. , EBELING H., MULLIS C.R., TULLY R.B.
	Astrophys. J., 662, 224-235 (2007)
	A systematic X-ray search for clusters of galaxies behind the Milky Way. II. The second CIZA subsample.
o	Table 2: <CIZA JHHMM.m+DDMM> N=57.
=E=	Catalogue in electronic form as J/ApJ/662/224
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CJ1
CJ1	(Caltech-Jodrell Bank, survey 1)
Write:	<<CJ1 HHMM+DDd>>
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	First ref. with objects from survey 1.
Ref:	=1995ApJS...98....1P
by	POLATIDIS A.G. , WILKINSON P.N., XU W., READHEAD A.C.S., PEARSON T.J., TAYLOR G.B., VERMEULEN R.C.
	Astrophys. J., Suppl. Ser., 98, 1-None (1995)
	The first Caltech-Jodrell Bank VLBI survey. I. Lambda = 18 centimeter observations of 87 sources.
o	<CJ1 HHMM+DDd> N=135
=E=	Catalogue in electronic form as J/ApJS/98/1
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CJ2
CJ2	(Caltech-Jodrell Bank, survey 2)
Write:	<<CJ2 HHMM+DDd>>
N:	193
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1994ApJS...95..345T
by	TAYLOR G.B. , VERMEULEN R.C., PEARSON T.J., READHEAD A.C.S., HENSTOCK D.R., BROWNE I.W.A., WILKINSON P.N.
	Astrophys. J., Suppl. Ser., 95, 345-369 (1994)
	The second Caltech-Jodrell bank VLBI survey. I. Observations of 91 of 193 sources.
o	<CJ2 HHMM+DDd> N=193
=E=	Catalogue in electronic form as J/ApJS/95/345
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CJ2010]
[CJ2010]	(Cargile+James, 2010)
Write:	<<[CJ2010] FF-NNN>>
N:	7200
Object:	* (SIMBAD class: Star)
Note:	CTIO SMARTS 1.0m telescope BVIc observations of IC 4665 (N=7200 stars in 9 fields).
in source:	IC 4665
Ref:	=2010AJ....140..677C
by	CARGILE P.A. , JAMES D.J.
	Astron. J., 140, 677-691 (2010)
	Employing a new, BVI_c photometric survey of IC 4665 to investigate the age of this young open cluster.
o	Table 3: <[CJ2010] FF-NNN> N=7200.
=E=	Catalogue in electronic form as <J/AJ/140/677/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CJ81]
[CJ81]	(Clark+Johnson, 1981)
Write:	<<[CJ81] Feature N>>
N:	5
Object:	Feature (SIMBAD class: Cloud)
Note:	N=5 features in the LDN 134-183 system.
in source:	LDN 134N
Ref:	=1981ApJ...247..104C
by	CLARK F.O. , JOHNSON D.R.
	Astrophys. J., 247, 104-111 (1981)
	The L134-L183-L1778 system of interstellar clouds.
o	Figs 1, 2: <[CJ81] Feature N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CJ87]
[CJ87]	(Cohen+Jones, 1987)
Write:	<<[CJ87] SVS 12 Knot A>> <<[CJ87] HH 30 Knot A>> <<[CJ87] HL Tau Knot A>> <<[CJ87] HH 34 Knot A>>
N:	7+6+12+5
Object:	Knot (SIMBAD class: PartofCloud = Part of Cloud)
Note:	Knots in the jet of HH objects. SVS 12 (= [SVS76] NGC 1333 12): N=7 knots (Nos A-G). HH 30: N=6 knots (Nos A-F). HL Tau: N=12 knots (Nos A-L). HH 34: N=5 knots (Nos A-E). Knots in HH 30 and HL Tau are also studued and cross-identified in [MRB88].
in source:	NGC 1333:[SVS76] NGC 1333 12 = [SVS76] NGC 1333 12
in source:	HH 30
in source:	V* HL Tau
in source:	HH 34
Ref:	=1987ApJ...321..846C
by	COHEN M. , JONES B.F.
	Astrophys. J., 321, 846-854 (1987)
	Observations of jets from low-luminosity stars. II. SVS 12, HH 30 near HL Tauri and HH 34.
o	Table 1: <[CJ87] SVS 12 Knot A> (Nos A-G). Table 2: <[CJ87] HH 30 Knot A> (Nos A-F). Table 3: <[CJ87] HL Tau Knot A> (Nos A-L). Table 4: <[CJ87] HH 34 Knot A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CJ92]
[CJ92]	(Cernis+Jasevicius, 1992)
Write:	<<[CJ92] SA N NN>>
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 2: * in SA 2: format 'SA 2 NN', N=26. Table 3: * in SA 4: format 'SA 4 NN', N=40. Table 4: * in SA 6: format 'SA 6 NN', N=48.
Ref:	=1992BaltA...1..168C
by	CERNIS K. , JASEVICIUS V.
	Baltic Astronomy, 1, 168-180 (1992)
	Photoelectric photometry of stars in the Vilnius system in Kapteyn Areas SA 2, 4, and 6.
o	Table 2: <[CJ92] SA 2 NN> N=26, Table 3: <[CJ92] SA 4 NN> N=40, Table 4: <[CJ92] SA 6 NN> N=48
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CJA2015]
[CJA2015]	(Calzetti+Johnson+Adamo+, 2015)
Write:	<<[CJA2015] NN>>
N:	11
Object:	Star Cluster (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST WFC3 photometric observations of N=11 star clusters in the starburst galaxy NGC 5253. Use of HST archival images.
in source:	NGC 5253
Ref:	=2015ApJ...811...75C
by	CALZETTI D. , JOHNSON K.E., ADAMO A., GALLAGHER III J.S., ANDREWS J.E., SMITH L.J., CLAYTON G.C., LEE J.C., SABBI E., UBEDA L., KIM H., RYON J.E., THILKER D., BRIGHT S.N., ZACKRISSON E., KENNICUTT R.C., DE MINK S.E., WHITMORE B.C., ALOISI A., CHANDAR R., CIGNONI M., COOK D., DALE D.A., ELMEGREEN B.G., ELMEGREEN D.M., EVANS A.S., FUMAGALLI M., GOULIERMIS D.A., GRASHA K., GREBEL E.K., KRUMHOLZ M.R., WALTERBOS R., WOFFORD A., BROWN T.M., CHRISTIAN C., DOBBS C., HERRERO A., KAHRE L., MESSA M., NAIR P., NOTA A., OSTLIN G., PELLERIN A., SACCHI E., SCHAERER D., TOSI M.
	Astrophys. J., 811, 75 (2015)
	The brightest young star clusters in NGC 5253.
o	Table 3: <[CJA2015] NN> N=11.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CJD2005]
[CJD2005]	(Casewell+Jameson+Dobbie, 2005) (Not yet in Simbad)
Write:	<<[CJD2005] JHHMMSS.ss+DDMMSS.s>>
Object:	Poss. BD* (SIMBAD class: BrownD*_Candidate = Brown Dwarf Candidate)
Note:	UKIRT UFTI and INT WFC observations of N=13 brown dwarf candidates in the Coma Berenices star cluster.
in source:	Cl Melotte 111 = NAME Coma Berenices Cluster
Ref:	=2005AN....326..991C
by	CASEWELL S.L. , JAMESON R.F., DOBBIE P.D.
	Astron. Nachr., 326, 991-995 (2005)
	New stellar and substellar candidate members of the Coma Berenices open star cluster.
o	Table 2: <[CJD2005] JHHMMSS.ss+DDMMSS.s> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CJD2006]
[CJD2006]	(Casewell+Jameson+Dobbie, 2006)
Write:	<<[CJD2006] JHHMMSS.ss+DDMMSS.s>>
N:	60
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Survey of Coma Berenices cluster (= Cl Melotte 111): 60 new candidate members are found. Use of USNO-B1.0 and 2MASS archival data.
Ref:	=2006MNRAS.365..447C
by	CASEWELL S.L. , JAMESON R.F., DOBBIE P.D.
	Mon. Not. R. Astron. Soc., 365, 447-453 (2006)
	New stellar members of the Coma Berenices open star cluster.
o	Table 2: <[CJD2006] JHHMMSS.ss+DDMMSS.s> N=60.
=E=	Catalogue in electronic form as J/MNRAS/365/447
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CJF
CJF	(Caltech-Jodrell bank Flat spectrum)
Write:	<<CJF BHHMM+DDd>>
N:	293
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 1: format 'BHHMM+DDd' given in 1950 eq. coord., and then col.(2) and (3) 2000 coordinates
Ref:	=1996ApJS..107...37T
by	TAYLOR G.B. , VERMEULEN R.C., READHEAD A.C.S., PEARSON T.J., HENSTOCK D.R., WILKINSON P.N.
	Astrophys. J., Suppl. Ser., 107, 37-68 (1996)
	A complete flux-density-limited VLBI survey of 293 flat-spectrum radio sources.
o	Table 1: <CJF BHHMM+DDd> N=293
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CJF89]
[CJF89]	(Ciardullo+Jacoby+Ford, 1989)
Write:	<<[CJF89] NGC NNNN NNN>> <<[CJF89] NGC NNNN a>>
N:	54+93+102+7+19+18
Object:	PN + * (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Table 2: PN in NGC 3377, format 'NGC 3377 NN', (Nos 1-54). Table 3: PN in NGC 3379, format 'NGC 3379 NN', (Nos 1-93). Table 4: PN in NGC 3384, format 'NGC 3384 NN', (Nos 1-102) Table 5: Reference * in NGC 3377, format 'NGC 3377 a', (Nos a-g). Reference * in NGC 3379, format 'NGC 3379 a', (Nos a-s). Reference * in NGC 3384, format 'NGC 3384 a', (Nos a-r). See also: Ford, [JCF89], [JCF90], [CJH91], [MCJ93], [JCH96], [FCJ97], [CJF98]
in source:	NGC 3377
in source:	NGC 3379
in source:	NGC 3384
Ref:	=1989ApJ...344..715C
by	CIARDULLO R. , JACOBY G.H., FORD H.C.
	Astrophys. J., 344, 715-725 (1989)
	Planetary nebulae as standard candles. IV. A test in the Leo I group.
o	Table 2: <[CJF89] NGC 3377 NN> N=54, Table 3: <[CJF89] NGC 3379 NN> N=93, Table 4: <[CJF89] NGC 3384 NNN> N=102, Table 5: <[CJF89] NGC 3377 a> (Nos a-g), <[CJF89] NGC 3379 a> (Nos a-s>, <[CJF89] NGC 3384 a> (Nos a-r) Tables 2, 3, 4 et 5 scannees par James Marcout.
=E=	Catalogue in electronic form as J/ApJ/344/715
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CJF98]
[CJF98]	(Ciardullo+Jacoby+Feldmeier+, 1989)
Write:	<<[CJF98] NGC 4478 N>> <<[CJF98] IC 3443 N>> <<[CJF98] Anon N>>
N:	7+1+1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=7 PN in NGC 4478, N=1 PN in IC 3443, and N=1 PN named 'Anon 1' Table 1: Numbering is following the numbering of [JCF90] in NGC 4486 See also: Ford, [CJF89], [JCF89], [JCF90], [CJH91], [MCJ93], [JCH96], [FCJ97]
in source:	NGC 4478
in source:	IC 3443
Ref:	=1998ApJ...492...62C
by	CIARDULLO R. , JACOBY G.H., FELDMEIER J.J., BARTLETT R.E.
	Astrophys. J., 492, 62-73 (1998)
	The planetary nebula luminosity function of M 87 and the intracluster stars of Virgo.
o	in NGC 4486, 10 PN from 1990ApJ...356..332J ([JCF90] NGC 4486) not found in this study.
o	Table 1: <[JCF90] NGC 4486 NNN> (Nos 56-339) added. Table 2: <[CJF98] NGC 4478 N> (Nos 1-7), <[CJF98] IC 3443 N> No. 1, <[CJF98] Anon N> No. 1.
=E=	Catalogue in electronic form as J/ApJ/492/62
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CJFN
CJFN	(Ciardullo+Jacoby+Ford+Neill)
*****	Avoid the usage of CJFN, prefer Ford
Origin	of the Acronym: L (1999ApJ...515..169J)
Details on Acronym: [CJH91]
[CJH91]	(Ciardullo+Jacoby+Harris, 1991)
Write:	<<[CJH91] NGC 1023 NNN>> <<[CJH91] NGC 891 NN>> <<[CJH91] NGC 1023 a>> <<[CJH91] NGC 891 a>>
N:	110+33+25+11
Object:	PN + * (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=110 PN in NGC 1023 Table 3: N=33 PN in NGC 891 Table 5: N=25 standard stars (Nos a-y) in NGC 1023, and N=11 standard stars (Nos a-k) in NGC 891 See also: Ford, [JCF89], [CJF89], [JCF90], [MCJ93], [JCH96], [FCJ97], [CJF98]
in source:	NGC 1023
in source:	NGC 891
Ref:	=1991ApJ...383..487C
by	CIARDULLO R. , JACOBY G.H., HARRIS W.E.
	Astrophys. J., 383, 487-497 (1991)
	Planetary nebulae as standard candles. VII. A test versus Hubble type in the NGC 1023 group.
o	Tables 2, 3, 5 not in SIMBAD
o	Table 2: <[CJH91] NGC 1023 NNN> (Nos 1-110). Table 3: <[CJH91] NGC 891 NN> (Nos 1-33). Table 5: <[CJH91] NGC 1023 a> (Nos a-y), <[CJH91] NGC 891 a> (Nos a-k).
=E=	Catalogue in electronic form as J/ApJ/383/487
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CJJ2010]
[CJJ2010]	(Cargile+James+Jeffries, 2010)
Write:	<<[CJJ2010] JCO-FFF-NNN>>
N:	8
Object:	* (SIMBAD class: Star)
Note:	Gemini GMOS spectroscopy and CTIO SMARTS observations of the open cluster Blanco 1.
in source:	Cl Blanco 1
Ref:	=2010ApJ...725L.111C
by	CARGILE P.A. , JAMES D.J., JEFFRIES R.D.
	Astrophys. J., 725L, 111-116 (2010)
	Identification of the lithium depletion boundary and age of the southern open cluster Blanco 1.
o	Table 1: <[CJJ2010] JCO-FFF-NNN> N=8 among (Nos F2-48 to F18-133).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CJK2015]
[CJK2015]	(Chun+Jung+Kang+, 2015)
Write:	<<[CJK2015] NNNNN>>
N:	446
Object:	AB* (SIMBAD class: AGB* = Asymptotic Giant Branch Star)
Note:	CFHT WIRCam photometric observations of N=446 asymptotic giant branch (AGB) stars of the dwarf irregular galaxy IC 1613.
in source:	IC 1613
Ref:	=2015A&A...578A..51C
by	CHUN S.-H. , JUNG M., KANG M., KIM J.-W., SOHN Y.-J.
	Astron. Astrophys., 578A, 51-51 (2015)
	Near-infrared photometric properties of asymptotic giant branch stars in the dwarf irregular galaxy IC 1613.
o	Table 2: <[CJK2015] NNNNN> N=446 among (Nos 475-22374).
=E=	Catalogue in electronic form as J/A+A/578/A51
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CJL94]
[CJL94]	(Coe+Jones+Lehto, 1994)
Write:	<<[CJL94] XA>>
N:	2
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observation of 1E 2259+58.6. Search for possible counterpart. N=2, (Nos XA-XB). XA = radioG 'EQ 2258+586' in Gregory, 1986 Can. J. of Phys. 64, p. 479
Ref:	=1994MNRAS.270..178C
by	COE M.J. , JONES L.R., LEHTO H.
	Mon. Not. R. Astron. Soc., 270, 178-182 (1994)
	A deep radio search for the counterpart to the enigmatic X-ray pulsar 1E 2259+586.
o	Fig.2: <[FHR82] A> (Nos W, X) added. Table 1: <[CJL94] XA> (Nos XA-XB).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CJM2014]
[CJM2014]	(Cannon+Johnson+McQuinn+, 2014)
Write:	<<[CJM2014] DDO 68 C>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLA (HI) and WIYN 0.9m telescope (optical) observations of N=1 galaxy companion of DDO 68. Use of archival HST, GALEX and SDSS data.
Ref:	=2014ApJ...787L...1C
by	CANNON J.M. , JOHNSON M., McQUINN K.B.W., ALFVIN E.D., BAILIN J., FORD H.A., GIRARDI L., HIRSCHAUER A.S., JANOWIECKI S., SALZER J.J., VAN SISTINE A., DOLPHIN A., ELSON E.C., KORIBALSKI B., MARIGO P., ROSENBERG J.L., ROSENFIELD P., SKILLMAN E.D., VENKATESAN A., WARREN S.R.
	Astrophys. J., 787L, 1 (2014)
	Discovery of a gas-rich companion to the extremely metal-poor galaxy DDO 68.
o	<[CJM2014] DDO 68 C> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CJS2003]
[CJS2003]	(Calchi Novati+Jetzer+Scarpetta+, 2003)
Write:	<<[CJS2003] CN>>
N:	5
Object:	Poss. Microlensing Event (SIMBAD class: LensingEv = (Micro)Lensing Event)
Stat:	is completely incorporated in Simbad
Note:	MDM observatory observations. See also [CIM2002].
in source:	M 31 = NGC 224
Ref:	=2003A&A...405..851C
by	CALCHI NOVATI S. , JETZER P., SCARPETTA G., GIRAUD-HERAUD Y., KAPLAN J., PAULIN-HENRIKSSON S., GOULD A.
	Astron. Astrophys., 405, 851-857 (2003)
	Microlensing towards M 31 with MDM data.
o	Table 1: Objects T1 to T5 = [CIM2002] 1 to 5, so T6 is designated as [CIM2002] 6 in SIMBAD.
o	Table 1: <[CIM2002] N> (No. 6) added. Tables 1, 2: <[CJS2003] CN> (Nos C1-C5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CJS2019]
[CJS2019]	(Chen+Johnson+Straka+, 2019)
Write:	<<[CJS2019] GNN>>
N:	12
Object:	G (SIMBAD class: Galaxy)
Note:	HST ACS, VLT MUSE, Magellan Clay telescope LDSS3 observations of N=12 galaxies in the field of SDSS J135726.27+043541.4. Use of DECaLS data.
Ref:	=2019MNRAS.484..431C
by	CHEN H.-W. , JOHNSON S.D., STRAKA L.A., ZAHEDY F.S., SCHAYE J., MUZAHID S., BOUCHE N., CANTALUPO S., MARINO R.A., WENDT M.
	Mon. Not. R. Astron. Soc., 484, 431-441 (2019)
	Characterizing circumgalactic gas around massive ellipticals at z ≃ 0.4 - III. The galactic environment of a chemically pristine Lyman limit absorber.
o	Fig. 2, Table 1: <[CJS2019] GNN> (Nos G1-G12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CJT2017]
[CJT2017]	(Chen+Jiang+Tamura+, 2017) (Not yet in Simbad)
Write:	<<[CJT2017] JDDD.dddddd+DD.dddddd>>
N:	356
Object:	* (SIMBAD class: Star)
Note:	IRSF 1.4m telescope SIRPOL observations of N=356 background stars in the field of the bubble [CPA2006] N4.
in source:	[CPA2006] N4
Ref:	=2017ApJ...838...80C
by	CHEN Z. , JIANG Z., TAMURA M., KWON J., ROMAN-LOPES A.
	Astrophys. J., 838, 80-80 (2017)
	A curved magnetic field in the ring-like shell of bubble N4.
o	Table 1: <[CJT2017] JDDD.dddddd+DD.dddddd> N=356.
=E=	Catalogue in electronic form as <J/ApJ/838/80/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CJT75]
[CJT75]	(Craine+Johnson+Tapia, 1975)
Write:	<<[CJT75] HHMM+DD A>>
N:	65
Object:	* (SIMBAD class: Star)
Note:	N=65 stars in the fields of 8 radio-sources, possible optical ID. Finding charts.
Ref:	=1975PASP...87..123C
by	CRAINE E.R. , JOHNSON K., TAPIA S.
	Publ. Astron. Soc. Pac., 87, 123-130 (1975)
	UBVr sequences and observations of optically identified radio sources.
o	Table II: <[CJT75] 1538+14 A> (Nos A-I), <[CJT75] 1656+05 A> (Nos A-E), <[CJT75] 1727+50 A> (Nos A-L), <[CJT75] 1749+09 A> (Nos A-I), <[CJT75] 2141+17 A> (Nos A-G), <[CJT75] 2254+07 A> (Nos A-J), <[CJT75] 2335+03 A> (Nos A-F), <[CJT75] 0219+42 A> (Nos A-G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CJV2018]
[CJV2018]	(Cantat-Gaudin+Jordi+Vallenari+, 2018)
Write:	<<Cl Gulliver NN>>
N:	60
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	N=60 Galactic star clusters identification based on the DR2 Gaia data release.
Ref:	=2018A&A...618A..93C
by	CANTAT-GAUDIN T. , JORDI C., VALLENARI A., BRAGAGLIA A., BALAGUER-NUNEZ L., SOUBIRAN C., BOSSINI D., MOITINHO A., CASTRO-GINARD A., KRONE-MARTINS A., CASAMIQUELA L., SORDO R., CARRERA R.
	Astron. Astrophys., 618A, 93-93 (2018)
	A Gaia DR2 view of the open cluster population in the Milky Way.
o	Table 1: <Cl Gulliver NN> (Nos 1-60).
=E=	Catalogue in electronic form as J/A+A/618/A93
Origin	of the Acronym: S = Created by Simbad, the CDS Database
History	of this Acronym: replaced by <	Details on Acronym: CK
CK	(Cometary Knot)
*****	Avoid the usage of CK, prefer [BO98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CK
CK	(Churchwell+Koornneef)
Write:	<<CK NN>>
N:	13
Object:	* (SIMBAD class: TTauri* = T Tauri Star)
Stat:	is completely incorporated in Simbad
in source:	NAME Serpens Cloud
Ref:	=1986ApJ...300..729C
by	CHURCHWELL E. , KOORNNEEF J.
	Astrophys. J., 300, 729-736 (1986)
	Pre-main-sequence stars in the Serpens molecular cloud.
o	<CK NN> (Nos 1-13).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CK
CK	(Cohen+Kuhi)
*****	Avoid the usage of CK, prefer CoKu
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CK2000]
[CK2000]	(Chengalur+Kanekar, 2000)
Write:	<<[CK2000] QSO JHHMM+DDMM abs N.NNNNN>> <<[CK2000] QSO JHHMM+DDMM abs N.NNNN>>
N:	5
Object:	DLA
Note:	GMRT 21cm line absorption observations in several QSOs.
Ref:	=2000MNRAS.318..303C
by	CHENGALUR J.N. , KANEKAR N.
	Mon. Not. R. Astron. Soc., 318, 303-308 (2000)
	Implications of 21-cm observations for damped Lyα systems.
o	Table 2: DLA which are not '[CK2000]' are already known with an other ID.
o	Table 2: <[CK2000] QSO JHHMM+DDMM abs N.NNNN>, <[CK2000] QSO JHHMM+DDMM abs N.NNNNN>, N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CK2002]
[CK2002]	(Cohen+Kneib, 2002)
Write:	<<[CK2002] {C\|O}MMSSs-MMSS>> <<[CK2002] A>>
N:	48+29+2
Object:	G + G in ClG (SIMBAD class: Galaxy)
Note:	Sample of 48 spectroscopically confirmed members of ClG J1347-1145, format 'CMMSSs-MMSS', and 29 background galaxies format 'OMMSSs-MMSS'. In the format, offset relative to RA = 13h and Dec = -11deg (2000). A lensed object is found in the field, and 2 possible counterparts A and B for this object.
in source:	ClG J1347-1145 = RX J1347.5-1145
Ref:	=2002ApJ...573..524C
by	COHEN J.G. , KNEIB J.-P.
	Astrophys. J., 573, 524-532 (2002)
	Losing weight: a Keck spectroscopic survey of the massive cluster of galaxies RX J1347-1145.
o	Table 1, text: <[CK2002] CMMSSs-MMSS> N=50. s-MMSS> N=29. Fig.1, text: <[CK2002] A> (Nos A-B) = <[CK2002] OMMSSs-MMSS> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CK2006]
[CK2006]	(CLewley+Kinman, 2006)
Write:	<<[CK2006] N>>
N:	8
Object:	Stellar Clump (SIMBAD class: Association = Association of Stars)
Stat:	is completely incorporated in Simbad
Note:	N=8 new clumps of BHB stars discovered in a catalogue of these stars compiled from the SDSS.
Ref:	=2006MNRAS.371L..11C
by	CLEWLEY L. , KINMAN T.D.
	Mon. Not. R. Astron. Soc., 371, 11-15 (2006)
	Spatial and velocity clumping in a Sloan Digital Sky Survey blue horizontal branch star catalogue.
o	Table 1: <[CK2006] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CK96]
[CK96]	(Caldwell+Kutner, 1996)
Write:	<<[CK96] 30Dor-Center>> <<[CK96] 30Dor-South>> <<[CK96] 30Dor-CNNA>> <<[CK96] 30Dor-S>> <<[CK96] 30Dor-SNN>> <<[CK96] N11-NNA>>
N:	2+21+4+30
Object:	MCld + Peak (SIMBAD class: MolCld = Molecular Cloud)
Note:	Table 1, col(1): N=21 Molecular clouds, in 3 regions in the region '[CK96] 30Dor-South': N=1 cloud '[CK96] 30Dor-S' in the region '[CK96] 30Dor-Center': N=8 clouds '[CK96] 30Dor-CNN' (+N=4 in text p. 617) among (Nos C01-C20) in the region N11 = 'LHA 120-N 11': N=12 clouds '[CK96] N11-NNA' among (Nos 01-13) Table 1, col(2): N=30 CO peaks associated with each source
in source:	Magellanic Clouds:LMC:NAME 30 Dor Nebula = NAME 30 Dor Nebula
in source:	Magellanic Clouds:LMC:LHA 120-N 11 = LHA 120-N 11
Ref:	=1996ApJ...472..611C
by	CALDWELL D.A. , KUTNER M.L.
	Astrophys. J., 472, 611-623 (1996)
	Star formation activity in the Large Magellanic Cloud: far-infrared emission from IRAS high-resolution data.
o	p. 612: <[CK96] 30Dor-Center>, <[CK96] 30Dor-South>. Table 1: <[CK96] 30Dor-S>, <[CK96] 30Dor-SNN> N=7, <[CK96] 30Dor-CNNA> N=13, <[CK96] N11-NNA> N=30. p. 617: <[CK96] 30Dor-CNN> N=4
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CK98]
[CK98]	(Chakrabarty+Kaspi, 1998)
Write:	<<[CK98] Star N>>
N:	5
Object:	* (SIMBAD class: Star)
Note:	Stars in the field of PSR 1706-44. Map in Fig.1
Ref:	=1998ApJ...498L..37C
by	CHAKRABARTY D. , KASPI V.M.
	Astrophys. J., 498, 37-40 (1998)
	A search for optical pulsations from two young southern pulsars.
o	Table 1, Fig.1: <[CK98] Star N> (Nos 1-6), No. 3 missing
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKB2000]
[CKB2000]	(Crawford+Kaspi+Bell, 2000)
Write:	<<[CKB2000] JHHMM+DDMM>>
N:	92
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Searched of 92 unidentified sources from NVSS and FIRST surveys.
Ref:	=2000AJ....119.2376C
by	CRAWFORD F. , KASPI V.M., BELL J.F.
	Astron. J., 119, 2376-2381 (2000)
	A search for submillisecond pulsations in unidentified FIRST and NVSS radio sources.
o	Table 1: <[CKB2000] JHHMM+DDMM> N=92.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKB2001]
[CKB2001]	(Clarke+Kronberg+Bohringer, 2001)
Write:	<<[CKB2001] JHHMM+DDda>>
N:	27
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA-ROSAT study of 16 ACO clusters: N=27 radio-sources.
Ref:	=2001ApJ...547L.111C
by	CLARKE T.E. , KRONBERG P.P., BOHRINGER H.
	Astrophys. J., 547, 111-114 (2001)
	A new radio-X-ray probe of galaxy cluster magnetic fields.
o	Table 1: <[CKB2001] JHHMM+DDda> N=27.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKB2005]
[CKB2005]	(Calzetti+Kennicutt+Bianchi+, 2005)
Write:	<<[CKB2005] IR-NN>> <<[CKB2005] xx-yy>>
N:	53+78
Object:	HII knot (SIMBAD class: HIIReg = HII Region)
Note:	Far-UV and Far-IR images of NGC 5194 from a combination of space-based (Spitzer, GALEX, HST) and ground-based data. In the format, the letters IR stand for Inner Region, and xx-yy indicate the background region where the aperture measurement is located.
in source:	NGC 5194 = M 51
Ref:	=2005ApJ...633..871C
by	CALZETTI D. , KENNICUTT R.C.Jr, BIANCHI L., THILKER D.A., DALE D.A., ENGELBRACHT C.W., LEITHERER C., MEYER M.J., SOSEY M.L., MUTCHLER M., REGAN M.W., THORNLEY M.D., ARMUS L., BENDO G.J., BOISSIER S., BOSELLI A., DRAINE B.T., GORDON K.D., HELOU G., HOLLENBACH D.J., KEWLEY L., MADORE B.F., MARTIN D.C., MURPHY E.J., RIEKE G.H., RIEKE M.J., ROUSSEL H., SHETH K., SMITH J.D., WALTER F., WHITE B.A., YI S., SCOVILLE N.Z., POLLETTA M., LINDLER D.
	Astrophys. J., 633, 871-893 (2005)
	Star formation in NGC 5194 (M51a): the panchromatic view from GALEX to Spitzer.
o	Table 1: <[CKB2005] IR-NN> (Nos IR-02 to IR-54), <[CKB2005] XX-YY) N=78.
=E=	Catalogue in electronic form as J/ApJ/633/871
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKB2007]
[CKB2007]	(Currie+Kenyon+Balog+, 2007)
Write:	<<[CKB2007] JHHMMSS.ss+DDMMSS.s>>
N:	30
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	MMT telescope Hectospec observations of the old clusters h and chi Persei. See also [CKB2008].
in source:	h Per Cluster = NGC 869
in source:	chi Per Cluster = NGC 884
Ref:	=2007ApJ...669L..33C
by	CURRIE T. , KENYON S.J., BALOG Z., BRAGG A., TOKARZ S.
	Astrophys. J., 669L, 33-36 (2007)
	Discovery of gas accretion onto stars in 13 Myr old h and χ Persei.
o	Table 1: <[CKB2007] JHHMMSS.ss+DDMMSS.s> N=30.
=E=	Catalogue in electronic form as J/ApJ/669/L33
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKB2008]
[CKB2008]	(Currie+Kenyon+Balog+, 2008)
Write:	<<[CKB2008] DD.dddd+DD.dddd>> <<[CKB2008] NN>>
N:	616+57
Object:	(IR) + Be* (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Spitzer MIPS observations of the double cluster h and chi Persei. See also [CKB2007].
in source:	h Per Cluster = NGC 869
in source:	chi Per Cluster = NGC 884
Ref:	=2008ApJ...672..558C
by	CURRIE T. , KENYON S.J., BALOG Z., RIEKE G., BRAGG A., BROMLEY B.
	Astrophys. J., 672, 558-574 (2008)
	The rise and fall of debris disks: MIPS observations of h and χ Persei and the evolution of Mid-IR emission from planet formation.
o	Table 1: <[CKB2008] DD.dddd+DD.dddd> N=616. Table 2: <[CKB2008] NN> (Nos 1-57).
=E=	Catalogue in electronic form as J/ApJ/672/558
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKB2012]
[CKB2012]	(Cassan+Kubas+Beaulieu+, 2012)
Write:	<<[CKB2012] OGLE-YYYY-BLG-NNN>>
N:	196
Object:	Lev (SIMBAD class: LensingEv = (Micro)Lensing Event)
Note:	N=196 microlensing events from the PLANET (Probing Lensing Anomalies Network) follow-up strategies of a representative sample of OGLE alerts (between 2002 and 2007).
Ref:	=2012Natur.481..167C
by	CASSAN A. , KUBAS D., BEAULIEU J.-P., DOMINIK M., HORNE K., GREENHILL J., WAMBSGANSS J., MENZIES J., WILLIAMS A., JORGENSEN U., UDALSKI A., BENNETT D.P., ALBROW M.D., BATISTA V., BRILLANT S., CALDWELL J.A.R., COLE A., COUTURES C., COOK H., DIETERS S., DOMINIS PRESTER D., DONATOWICZ J., FOUQUE P., HILL K., KAINS N., KANE S., MARQUETTE J.-B., MARTIN R., POLLARD K.R., SAHU K.C., VINTER C., WARREN D., WATSON B., ZUB M., SUMI T., SZYMANSKI M.K., KUBIAK M., POLESKI R., SOSZYNSKI I., ULACZYK K., PIETRZYNSKI G., WYRZYKOWSKI L.
	Natur, 481, 167-169 (2012)
	One or more bound planets per Milky Way star from microlensing observations.
o	Table S1: <[CKB2012] OGLE-YYYY-BLG-NNN> N=196.
=E=	Catalogue in electronic form as J/other/Nat/481.167
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKC2010]
[CKC2010]	(Cseh+Kaaret+Corbel+, 2010)
Write:	<<[CKC2010] NN>>
N:	18
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS observations of the globular cluster NGC 6388.
in source:	NGC 6388
Ref:	=2010MNRAS.406.1049C
by	CSEH D. , KAARET P., CORBEL S., KORDING E., CORIAT M., TZIOUMIS A., LANZONI B.
	Mon. Not. R. Astron. Soc., 406, 1049-1054 (2010)
	Radio observations of NGC 6388: an upper limit on the mass of its central black hole.
o	Table 1: <[CKC2010] NN> (Nos 1-18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKF95]
[CKF95]	(Calzetti+Kinney+Ford+, 1995)
Write:	<<[CKF95] Em NNN>> <<[CKF95] HII NNN>>
N:	153+279
Object:	Em* + H-alpha (SIMBAD class: EmLine* = Emission-line Star)
Note:	Table 1: N=153 line emitting point-like sources, format 'Em NNN', (Nos 1-153) Table 2: N=279 compact HII regions, format 'HII NNN', (Nos 1-279)
in source:	M 33 = NGC 598
Ref:	=1995AJ....110.2739C
by	CALZETTI D. , KINNEY A.L., FORD H., DOGGETT J., LONG K.S.
	Astron. J., 110, 2739-2746 (1995)
	An atlas of H-α emitting regions in M33: a systematic search for SS433 star candidates.
o	In tables, ID of the source within the field (col. 3) should not be used. Cross-id: MC = [MC83], MCMS, SNR HHMMSS+DDMMm
o	Table 1: <[CKF95] Em NNN> (Nos 1-153), Table 2: <[CKF95] HII NNN> (Nos 1-279)
=E=	Catalogue in electronic form as J/AJ/110/2739
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKG2005]
[CKG2005]	(Cenko+Kulkarni+Gal-Yam+, 2005)
Write:	<<[CKG2005] Host G>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck LRIS observations of the host galaxy of GRB050416.
Ref:	=2005GCN..3542....1C
by	CENKO S.B. , KULKARNI S.R., GAL-YAM A., BERGER E.
	GRB Coordinates Network, Circular Service, 3542, 1-None (2005)
	GRB 050416(a): host galaxy redshift determination.
o	<[CKG2005] Host G> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKM99]
[CKM99]	(Conti+Kennefick+Martini+, 1999)
Write:	<<[CKM99] NNNN>>
N:	41
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
in source:	NAME HDFN
Ref:	=1999AJ....117..645C
by	CONTI A. , KENNEFICK J.D., MARTINI P., OSMER P.S.
	Astron. J., 117, 645-657 (1999)
	Quasar candidates in the Hubble Deep Field.
o	Table 2: <[CKM99] NNNN> N=41 among (Nos 94-3595).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKO2017]
[CKO2017]	(Coleman+King+Oguri+, 2017) (Not yet in Simbad)
Write:	<<[CKO2017] aN>>
N:	18+44
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	HST ACS and WFC observations N=44 lensed images of 18 background objects in the field of the two ACO 2146 subclusters.
Ref:	=2017MNRAS.464.2469C
by	COLEMAN J.E. , KING L.J., OGURI M., RUSSELL H.R., CANNING R.E.A., LEONARD A., SANTANA R., WHITE J.A., BAUM S.A., CLOWE D.I., EDGE A., FABIAN A.C., McNAMARA B.R., O'DEA C.P.
	Mon. Not. R. Astron. Soc., 464, 2469-2480 (2017)
	The mass distribution of the unusual merging cluster Abell 2146 from strong lensing.
o	Fig. 2, Tables A1-A2: <[CKO2017] a> (Nos a-n, p-s), <[CKO2017] aN> N=44.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKP2005]
[CKP2005]	(Chochol+Katysheva+Pribulla+, 2005) (Not yet in Simbad)
Write:	<<[CKP2005] N>>
N:	6
Object:	* (SIMBAD class: Star)
Note:	Comparison stars in the field of V475 Sct.
Ref:	=2005CoSka..35..107C
by	CHOCHOL D. , KATYSHEVA N.A., PRIBULLA T., SCHMIDTOBREICK L., SHUGAROV S.Y., SKODA P., SLECHTA M., VITTONE A.A., VOLKOV I.M.
	Contr. Astron. Obs. Skalnate Pleso, 35, 107-129 (2005)
	Photometric and spectroscopic variability of the slow nova V475 Sct (Nova Scuti 2003).
o	Table 1, Fig.1: <[CKP2005] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKR2003]
[CKR2003]	(Chini+Kampgen+Reipurth+, 2003)= (MMS)
Write:	<<[CKR2003] MMS NN>>
N:	25
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	SIMBA (SEST Imaging Bolometer Array) observations on SEST. Map fo CrA molecular Cloud at 1.2mm.
in source:	NAME R CrA Cloud
Ref:	=2003A&A...409..235C
by	CHINI R. , KAEMPGEN K., REIPURTH B., ALBRECHT M., KREYSA E., LEMKE R., NIELBOCK M., REICHERTZ L.A., SIEVERS A., ZYLKA R.
	Astron. Astrophys., 409, 235-244 (2003)
	SIMBA observations of the R Corona Australis molecular cloud.
o	Fig. 3 : VLA 10A, 10B =[TS84] IRS 7A, 7B. Object TIMMI = [TS84] IRS 7. Table 2 : NE and SW jaws not in SIMBAD.
o	Table 1: <[CKR2003] MMS NN> (Nos 1-25).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKR2007]
[CKR2007]	(Currie+Kenyon+Rieke+, 2007)
Write:	<<[CKR2007] N>>
N:	8
Object:	* in stellar cluster (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	MMT and 1.5m Tillinghast telescope at F.L. Whipple Observatory spectroscopic observations of the double cluster h and chi Persi. Analysis of 8 sources with strong MIR excesses in [CBK2007b].
in source:	NAME h Per = NGC 869
in source:	NAME khi Per = NGC 884
Ref:	=2007ApJ...663L.105C
by	CURRIE T. , KENYON S.J., RIEKE G., BALOG Z., BROMLEY B.C.
	Astrophys. J., 663L, 105-108 (2007)
	Terrestrial zone debris disk candidates in h and χ Persei.
o	Table 1: <[CKR2007] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKR2013]
[CKR2013]	(Cioni+Kamath+Rubele+, 2013)
Write:	<<[CKR2013] VMC JHHMMSS.ss+DDMMSS.s>>
N:	117
Object:	Q
Note:	VMC (VISTA Magellanic Clouds survey) known quasars behind the Magellanic system.
in source:	NAME LMC
in source:	NAME SMC
Ref:	=2013A&A...549A..29C
by	CIONI M.-R.L. , KAMATH D., RUBELE S., VAN LOON J.T., WOOD P.R., EMERSON J.P., GIBSON B.K., GROENEWEGEN M.A.T., IVANOV V.D., MISZALSKI B., RIPEPI V.
	Astron. Astrophys., 549A, 29-29 (2013)
	The VMC survey. VI. Quasars behind the Magellanic system.
o	In ref list Kozlowski et Al. 2011, ApJ, 194, 22 is a misprint for Kozlowski et Al. 2011, ApJS, 194, 22. Fig MACHO 78.8588.788 not identified.
o	Table 2 <[CKR2013] VMC JHHMMSS.ss+DDMMSS.s> N=117
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKR2016]
[CKR2016]	(Caminha+Karman+Rosati+, 2016)
Write:	<<[CKR2016] LAB>> <<[CKR2016] AN>>
N:	1+9
Object:	Lyman Alpha Blob + LeI (SIMBAD class: EmObj = Emission Object)
Note:	VLT MUSE observations of N=1 Lyman Alpha Blob, lensed the galaxy cluster ACO S 1063 into N=9 multiple images.
in source:	RXC J2248.7-4431 = ACO S 1063
Ref:	=2016A&A...595A.100C
by	CAMINHA G.B. , KARMAN W., ROSATI P., CAPUTI K.I., ARRIGONI BATTAIA F., BALESTRA I., GRILLO C., MERCURIO A., NONINO M., VANZELLA E.
	Astron. Astrophys., 595A, 100-100 (2016)
	Discovery of a faint, star-forming, multiply lensed, Lyman-α blob.
o	Text: <[CKR2016] LAB> N=1. Figs 1-2, Table 1: <[CKR2016] AN> (Nos A1-A3, B1-B3, C1-C3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKS2000]
[CKS2000]	(Csak+Kiss+Szabo+, 2000)
Write:	<<[CKS2000] VNN>>
N:	30
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Ref:	=2000IBVS.4875....1C
by	CSAK B. , KISS L.L., SZABO G., SARNECZKY K., SZILADI K.
	IAU Inform. Bull. Var. Stars, 4875, 1-None (2000)
	New field variable stars I.
o	<[CKS2000] VNN> (Nos V1-V11).
Ref:	=2000IBVS.4881....1C
by	CSAK B. , KISS L.L., SZILADI K., SARNECZKY K., SZABO G.
	IAU Inform. Bull. Var. Stars, 4881, 1-4 (2000)
	New field variable stars II.
o	<[CKS2000] VNN> (Nos V12-V17).
Ref:	=2000IBVS.4989....1C
by	CSAK B. , KISS L.L., SZABO G., SZILADI K., SARNECZKY K.
	IAU Inform. Bull. Var. Stars, 4989, 1-None (2000)
	New field variable stars III.
o	<[CKS2000] VNN> (Nos V18-V30).
Ref:	=2001IBVS.5049....1C
by	CSAK B. , KISS L.L., KOVACS D., MESZAROS S., SARNECZKY K., SZEKELY P.
	IAU Inform. Bull. Var. Stars, 5049, 1-None (2001)
	Two new contact binary stars.
o	<[CKS2000] VNN> (Nos V31-V32).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKS2001]
[CKS2001]	(Czoske+Kneib+Soucail+, 2001)= (Cz01)
Write:	<<[CKS2001] NNN>>
N:	688
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	CFHT-WHT spectroscopic survey of ClG 0024+1652.
in source:	ClG 0024+1652 = HMS 0024+1654
Ref:	=2001A&A...372..391C
by	CZOSKE O. , KNEIB J.-P., SOUCAIL G., BRIDGES T.J., MELLIER Y., CUILLANDRE J.-C.
	Astron. Astrophys., 372, 391-405 (2001)
	A wide-field spectroscopic survey of the cluster of galaxies Cl 0024+1654. I. The catalogue.
o	Table 4: <[CKS2001] NNN> (Nos 1-688).
=E=	Catalogue in electronic form as J/A+A/372/391
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKS2003]
[CKS2003]	(Candia+Krisciunas+Suntzeff+, 2003) (Not yet in Simbad)
Write:	<<[CKS2003] NN>>
N:	11
Object:	* (SIMBAD class: Star)
Note:	N=11 comparison stars near SN 2000CX.
Ref:	=2003PASP..115..277C
by	CANDIA P. , KRISCIUNAS K., SUNTZEFF N.B., GONZALEZ D., ESPINOZA J., LEITON R., REST A., SMITH R.C., CUADRA J., TAVENNER T., LOGAN C., SNIDER K., THOMAS M., WEST A.A., GONZALEZ G., GONZALEZ S., PHILLIPS M.M., HASTINGS N.C., McMILLAN R.
	Publ. Astron. Soc. Pac., 115, 277-294 (2003)
	Optical and infrared photometry of the unusual type Ia supernova 2000cx.
o	Fig.1, Table 2: <[CKS2003] NN> (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKS2006]
[CKS2006]	(Covone+Kneib+Soucail+, 2006)
Write:	<<[CKS2006] NN>> <<[CKS2006] AN>> <<[CKS2006] Ra>>
N:	38+10+3
Object:	G + Grav. lensed image (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT VIMOS-IFU survey of the lensing cluster ACO 2667: N=38 galaxies in the clusters, N=10 multiple and N=3 single lensed systems and magnified background galaxies. See also [CAD2006].
in source:	ACO 2667
Ref:	=2006A&A...456..409C
by	COVONE G. , KNEIB J.-P., SOUCAIL G., RICHARD J., JULLO E., EBELING H.
	Astron. Astrophys., 456, 409-420 (2006)
	VIMOS-IFU survey of z~0.2 massive galaxy clusters. I. Observations of the strong lensing cluster Abell 2667.
o	Table 1: <[CKS2006] NN> (Nos 1-38). Table 2: <[CKS2006] AN> (Nos A1-A3, B1-B3, C1-C2, D1-D2), <[CKS2006] Ra> (Nos Ra, Rb, RC).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKS2007]
[CKS2007]	(CHurchill+Kacprzak+Steidel+, 2007)
Write:	<<[CKS2007] GN>>
Object:	G in Pair (SIMBAD class: GinPair = Galaxy in Pair of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of the field of Ton 153.
Ref:	=2007ApJ...661..714C
by	CHURCHILL C.W. , KACPRZAK G.G., STEIDEL C.C., EVANS J.L.
	Astrophys. J., 661, 714-718 (2007)
	On the heterogeneity of metal-line and Lyα absorption in galaxy ``Halos'' at z ~ 0.7.
o	Fig.1: <[CKS2007] GN> (Nos G1-G2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKS2019]
[CKS2019]	(Cantat-Gaudin+Krone-Martins+Sedaghat+, 2019)
Write:	<<[CKS2019] COIN-Gaia NN>> <<[CKS2019] COIN-Gaia_NN>> (not recognised by Simbad, but found in literature)
N:	41
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	N=41 open star clusters in Gaia DR2, as part of the Cosmostatistics Initiative (COIN): https://cosmostatistics-initiative.org
Ref:	=2019A&A...624A.126C
by	CANTAT-GAUDIN T. , KRONE-MARTINS A., SEDAGHAT N., FARAHI A., DE SOUZA R.S., SKALIDIS R., MALZ A.I., MACEDO S., MOEWS B., JORDI C., MOITINHO A., CASTRO-GINARD A., ISHIDA E.E.O., HENEKA C., BOUCAUD A., TRINDADE A.M.M.
	Astron. Astrophys., 624A, 126-126 (2019)
	Gaia DR2 unravels incompleteness of nearby cluster population: new open clusters in the direction of Perseus.
o	Table A.1: <[CKS2019] COIN-Gaia NN> (Nos 1-41).
=E=	Catalogue in electronic form as <J/A+A/624/A126/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKS91]
[CKS91]	(Caldwell+Keane+Schechter, 1991)
Write:	<<[CKS91] HHMMm-DDMM>>
N:	2422
Object:	V* (SIMBAD class: Variable* = Variable Star)
Ref:	=1991AJ....101.1763C
by	CALDWELL J.A.R. , KEANE M.J., SCHECHTER P.L.
	Astron. J., 101, 1763-1787 (1991)
	A scanned CCD search for Cepheids and other variables in Crux and Centaurus.
o	<[CKS91] HHMMm-DDMM> N=2422
=E=	Catalogue in electronic form as II/162
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKS96]
[CKS96]	(Currie+Kissell+Shaya+, 1996)
Write:	<<[CKS96] A>>
N:	3
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	ESO 3.6m telescope SHARP II NICMOS observations of NGC 6611 using adaptive optics (ADONIS). 3 Objects are found near the star NGC 6611 367.
in source:	M 16 = Eagle Nebula = NGC 6611
Ref:	=1996Msngr..86...31C
by	CURRIE D. , KISSELL K., SHAYA E., AVIZONIS P., DOWLING D., BONACCINI D.
	The Messenger, 86, 31-36 (1996)
	Star formation in NGC 6611 with ADONIS and Hubble.
o	Fig.7: <[CKS96] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKT2009]
[CKT2009]	(Chiboucas+Karachentsev+Tully, 2009)
Write:	<<[CKT2009] dJHHMM+DD>> <<[CKT2009] dHHMM+DD>> (not recognised by Simbad, but found in literature)
N:	22
Object:	Poss. Dwarf G (SIMBAD class: Galaxy)
Note:	CFHT MegaCam observations to search for new possible dwarf galaxies in the M 81 group.
in source:	NAME M 81 GROUP
Ref:	=2009AJ....137.3009C
by	CHIBOUCAS K. , KARACHENTSEV I.D., TULLY R.B.
	Astron. J., 137, 3009-3037 (2009)
	Discovery of new dwarf galaxies in the M81 group.
o	Table 1: <[CKT2009] dJHHMM+DD> N=22.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKT2015]
[CKT2015]	(Cummings+Kalirai+Tremblay+, 2015)
Write:	<<[CKT2015] NGC NNNN WDNN>>
N:	19+9+10
Object:	Poss. WD (SIMBAD class: WhiteDwarf_Candidate = White Dwarf Candidate)
Note:	Keck I LRIS spectroscopy of N=19 white dwarfs in the rich open cluster NGC 2099 (M37) and NGC 2323 (M 50).
in source:	M 37 = NGC 2099
in source:	M 50 = NGC 2323
Ref:	=2015ApJ...807...90C
by	CUMMINGS J.D. , KALIRAI J.S., TREMBLAY P.-E., RAMIREZ-RUIZ E.
	Astrophys. J., 807, 90 (2015)
	Initial-final mass relation for 3 to 4 M_☉ progenitors of white dwarfs from the single cluster NGC 2099.
o	Table 1: <[CKT2015] NGC 2099 WDNN> N=19 among (Nos 1-24).
Ref:	=2016ApJ...820L..18C
by	CUMMINGS J.D. , KALIRAI J.S., TREMBLAY P.-E., RAMIREZ-RUIZ E., BERGERON P.
	Astrophys. J., 820L, 18 (2016)
	An ultramassive 1.28 M_☉ white dwarf in NGC 2099.
o	Table 1: <[CKT2015] NGC 2099 WDNN> N=9 (Nos 25-33) added.
Ref:	=2016ApJ...818...84C
by	CUMMINGS J.D. , KALIRAI J.S., TREMBLAY P.-E., RAMIREZ-RUIZ E.
	Astrophys. J., 818, 84 (2016)
	Two massive white dwarfs from NGC 2323 and the initial-final mass relation for progenitors of 4 to 6.5 M.
o	Table 1,3: <[CKT2015] NGC 2323 WDNN> N=10 among (Nos 7-38).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CKV
CKV	(Corbin+Korista+Vacca)
*****	Avoid the usage of CKV, prefer [CKV93]
Origin	of the Acronym: L (1997A&A...325...98S)
Details on Acronym: [CKV93]
[CKV93]	(Corbin+Korista+Vacca, 1993)= (CKV)
Write:	<<[CKV93] A>>
N:	3
Object:	Region (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=3 starburst regions (Nos A-C) in the WR galaxy 'Hen 2-10'. See also , [KJ99], [MEF99].
in source:	Hen 2-10
Ref:	=1993AJ....105.1313C
by	CORBIN M.R. , KORISTA K.T., VACCA W.D.
	Astron. J., 105, 1313-1317 (1993)
	Imaging of the Wolf-Rayet galaxy He 2-10.
o	Table 1, Fig.2: <[CKV93] A> (Nos A-B).
Ref:	=1997A&A...325...98S
by	SAUVAGE M. , THUAN T.X., LAGAGE P.O.
	Astron. Astrophys., 325, 98-108 (1997)
	10 µm imaging and HI observations of the Blue Compact Dwarf galaxy He 2-10.
o	(Erratum) Erratum vol. 333, p. 1143
o	<[CKV93] A> (No. C) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKV94]
[CKV94]	(Chiar+Kutner+Verter+, 1994)
Write:	<<[CKV94] NN>>
N:	34
Object:	Cloud (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
in source:	NAME Sct Arm
Ref:	=1994ApJ...431..658C
by	CHIAR J.E. , KUTNER M.L., VERTER F., LEOUS J.
	Astrophys. J., 431, 658-673 (1994)
	A comparison of CO (J=1 ⟶0) and CO (J=2 ⟶1) emission in the Milky Way molecular ring.
o	<[CKV94] NN> N=34
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKW87]
[CKW87]	(Chini+Krugel+Wargau, 1987)
Write:	<<[CKW87] HHMMSS.s+DDMMSS>>
N:	66
Object:	HII (SIMBAD class: HIIReg = HII Region)
Ref:	=1987A&A...181..378C
by	CHINI R. , KRUGEL E., WARGAU W.
	Astron. Astrophys., 181, 378-382 (1987)
	Dust emission and star formation in compact HII regions.
o	Table 1: <[CKW87] HHMMSS.s+DDMMSS> N=66
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CKW92]
[CKW92]	(Chini+Krugel+Wargau, 1992)= (IRS)
Write:	<<[CKW92] IRS NN>>
N:	71
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	ESO 2.2 m telescope and SAAO 1.9 m telescope observations. 71 mostly unknown IR sources towards NGC 6611 = M 16.
in source:	M 16 = Eagle Nebula = NGC 6611
Ref:	=1992A&A...265...45C
by	CHINI R. , KRUGEL E., WARGAU W.F.
	Astron. Astrophys., 265, 45-54 (1992)
	A cluster of infrared sources towards M 16.
o	Table I: <[CKW92] IRS NN> (Nos 1-71).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Cl
Cl	(Claria) (Not yet in Simbad)
*****	Avoid the usage of Cl, prefer [C74]
Origin	of the Acronym: L (1999MNRAS.310..210S)
Details on Acronym: CL
CL	(Clark Lake obs.) (Not yet in Simbad)
*****	Avoid the usage of CL, prefer [VE75]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cl
Cl	(Cluster of G)
*****	Avoid the usage of Cl, prefer ClG
Details on Acronym: Cl
Cl	(Cluster)
*****	Avoid the usage of Cl, prefer HMS
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CL
CL	(Cygnus Loop)
*****	Avoid the usage of CL, prefer [KWH73]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cl
Cl	(Cluster)
*****	Avoid the usage of Cl, prefer [LP96]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CL
CL	(Cluster)
*****	Avoid the usage of CL, prefer [PLO2002]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cl
Cl	(Cluster)
*****	Avoid the usage of Cl, prefer [ZND97]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: *Cl NGC 5139 S**
*Cl NGC 5139 S**	(Seitzer)
Write:	<<*Cl NGC 5139 S** NNN>>
N:	20
Object:	*inCl
Rem:	Seitzer, 1983, PhD thesis, Univ. of Virginia
Ref:	=1996ApJ...462..241N
by	NORRIS J.E. , FREEMAN K.C., MIGHELL K.J.
	Astrophys. J., 462, 241-254 (1996)
	The giant branch of ω Centauri. V. The calcium abundance distribution.
o	Tables 1+3, col(1): NNN are <NGC 5139 NNN> in SIMBAD, 7NNN are <Cl* NG C 5139 S NNN> in SIMBAD, 8NNN are <Cl* NGC 5139 MAR NNN> in SIMBAD, 9NNN from the present work.
o	Tables 1, 3: <[NFM96] 9NNN> N=74 among (Nos 9002-9227). Table 1: <Cl* NGC 5139 S NNN> N=20 among (Nos 6-903), <Cl* NGC 5139 MAR NNN> N=5 among (Nos 181-187) added.
Details on Acronym: *Cl NGC 6121 MVP**
*Cl NGC 6121 MVP**	(Marino+Villanova+Piotto+, 2008)
Write:	<<*Cl NGC 6121 MVP** NNNNN>>
N:	105+23
Object:	*inCl
Stat:	is completely incorporated in Simbad
Ref:	=2008A&A...490..625M
by	MARINO A.F. , VILLANOVA S., PIOTTO G., MILONE A.P., MOMANY Y., BEDIN L.R., MEDLING A.M.
	Astron. Astrophys., 490, 625-640 (2008)
	Spectroscopic and photometric evidence of two stellar populations in the Galactic globular cluster NGC 6121 (M4).
o	Table 8: <Cl* NGC 6121 MVP NNNNN> N=105 among (Nos 5359-48895).
Ref:	=2011A&A...535A..31V
by	VILLANOVA S. , GEISLER D.
	Astron. Astrophys., 535A, 31-31 (2011)
	Bimodality of light and s-elements in M4 (NGC 6121). A hint for the massive main-sequence star pollution scenario.
o	Table 1: <Cl* NGC 6121 MVP NNNNN> N=23 among (Nos 907-67553) added.
=E=	Catalogue in electronic form as J/A+A/490/625
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CL2003]
[CL2003]	(Chen+Lanzetta, 2003)
Write:	<<[CL2003] AO 0235+164 N>> <<[CL2003] EX 0302-2223 N>> <<[CL2003] PKS 0439-433 N>> <<[CL2003] HE 1122-1649 NN>> <<[CL2003] PKS 1127-145 N>> <<[CL2003] QSO JHHMM+DDMM abs N.NNN>> <<[CL2003] QSO JHHMM+DDMM abs N.NNNN>>
N:	4+7+3+10+8+7
Object:	G + Absorber (SIMBAD class: Galaxy)
Note:	Las Campanas observations. Study of galaxies in 5 fields, and of DLAs (Table 7). Some of these DLAs are already known.
Ref:	=2003ApJ...597..706C
by	CHEN H.-W. , LANZETTA K.M.
	Astrophys. J., 597, 706-729 (2003)
	The nature of damped Lyα absorbing galaxies at z ≤ 1: a photometric redshift survey of damped Lyα absorbers.
o	Table 1: AO 0235+164 and EX 0302-2223 are repectively AO 0235+16 and EXO 0302-223 in SIMBAD. Table 7: ALS which are not with '[CL2003]' ID are already known in SIMBAD.
o	Fig.2, Table 2: <[CL2003] AO 0235+164 N> (Nos 1-4). Fig.4, Table 3: <[CL2003] EX 0302-2223 N> (Nos 1-7). Fig.6, Table 4: <[CL2003] PKS 0439-433 N> (Nos 1-3). Fig.8, Table 5: <[CL2003] HE 1122-1649 NN> (Nos 1-10). Fig.10, Table 6: <[CL2003] PKS 1127-145 N> (Nos 1-8). Table 7: <[CL2003] QSO JHHMM+DDMM abs N.NNN>, <[CL2003] QSO JHHMM+DDMM abs N.NNNN>, N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CL2012]
[CL2012]	(Castro-Rodriguez+Lopez-Corredoira, 2012)= (UDS)
Write:	<<[CL2012] UDS NNNNN>>
N:	20
Object:	G (SIMBAD class: Galaxy)
Note:	N=20 old galaxies within very high-redshift extremely red objects (EROs). Use of data from the UKIDSS Ultra Deep Survey (UDS), Subaru/XMM-Newton Deep Survey (SXDS), and Spitzer SWIRE survey.
Ref:	=2012A&A...537A..31C
by	CASTRO-RODRIGUEZ N. , LOPEZ-CORREDOIRA M.
	Astron. Astrophys., 537A, 31-31 (2012)
	The age of extremely red and massive galaxies at very high redshift.
o	Table 1: <[CL2012] UDS NNNNN> N=20 among (nos 1559-93574).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CL2013]
[CL2013]	(Clem+Landolt, 2013) (Not yet in Simbad)
Write:	<<[CL2013] JLNNN NNNN>> <<[CL2013] TPhe NNN>> <<[CL2013] Feige24 NN>> <<[CL2013] PGHHMM+DDd NNNN>> <<[CL2013] SANNN NNNN>> <<[CL2013] SANNN FN NNN>> <<[CL2013] MCTHHMM+DDMM NNN>> <<[CL2013] LB1735 NNN>> <<[CL2013] GDNNN NNNN>> <<[CL2013] LSENNN NNNN>> <<[CL2013] LSSNNN NNNN>> <<[CL2013] RuNNN NNNN>> <<[CL2013] WDHHMM+DDd NNNN>> <<[CL2013] JHHMMSS+DDMMSS NNNN>> <<[CL2013] GFFF-NNN NNN>> <<[CL2013] MarkA NNN>>
N:	∼45000
Object:	* (SIMBAD class: Star)
Note:	CTIO 1.0m telescope UBVRI photometry of N∼45000 stars distributed among 60 different fields centered on the celestial equator and at δ∼50°.
Ref:	=2013AJ....146...88C
by	CLEM J.L. , LANDOLT A.U.
	Astron. J., 146, 88 (2013)
	Faint UBVRI standard star fields.
o	Table 7: <[CL2013] JLNNN NNNN>, <[CL2013] TPhe NNN>, <[CL2013] PGHHMM+DDd NNN>, <[CL2013] Feige24 NN>, <[CL2013] SANNN NNNN>, <[CL2013] SANNN FN NN>, <[CL2013] MCTHHMM+DDMM NNN>, <[CL2013] LB1735 NNN>, <[CL2013] GDNNN NNNN>, <[CL2013] LSENNN NNNN>, <[CL2013] LSSNNN NNNN>, <[CL2013] RuNNN NNNN>, <[CL2013] WDHHMM+DDd NNNN>, <[CL2013] JHHMMSS+DDMMSS NNNN>, <[CL2013] GFFF-NNN NNN>, <[CL2013] MarkA NNN>, N~45000.
=E=	Catalogue in electronic form as <J/AJ/146/88/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CL2016]
[CL2016]	(Clem+Landolt, 2016)
Write:	<<[CL2016] JHHMMSS+DDMMSS NNN>> <<[CL2016] GDNNN NNN>>
N:	2125
Object:	* (SIMBAD class: Star)
Note:	KPNO 2.1m telescope photometric observations of N=2125 standard star sequences around the sky at ∼ 50° declination. See also [L92b] and [L2007].
Ref:	=2016AJ....152...91C
by	CLEM J.L. , LANDOLT A.U.
	Astron. J., 152, 91-91 (2016)
	Faint UBVRI standard star fields at +50° declination.
o	Table 6: <[CL2016] GDNNN NNN>, [CL2016] JHHMMSS+DDMMSS> N=2125.
=E=	Catalogue in electronic form as J/AJ/152/91
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CL95]
[CL95]	(Castets+Langer, 1995)
Write:	<<[CL95] OMC-3 A>>
N:	3
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Tables 3, 4: N=3 OMC 3 cores A, B, C
in source:	OMC:OMC 3 = OMC 3
Ref:	=1995A&A...294..835C
by	CASTETS A. , LANGER W.D.
	Astron. Astrophys., 294, 835-854 (1995)
	Physical properties of the OMC-2 and OMC-3 cores from CS and C^{18}O observations.
o	Tables 3, 4: <[CL95] OMC-3 A> N=3
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CLANS
CLANS	(Chandra Lockman Area North Survey)
Write:	<<CLANS NNN>>
N:	789
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-I and CFHT MegaCam-/WIRCam observations in the Lockman Hole.
in source:	NAME Lockman Hole
Ref:	=2008ApJS..179....1T
by	TROUILLE L. , BARGER A.J., COWIE L.L., YANG Y., MUSHOTZKY R.F.
	Astrophys. J., Suppl. Ser., 179, 1-18 (2008)
	The OPTX project. I. The flux and redshift catalogs for the CLANS, CLASXS, and CDF-N fields.
o	Tables 4,5: <CLANS NNN> (Nos 1-761).
Ref:	=2009ApJ...703.2160T
by	TROUILLE L. , BARGER A.J., COWIE L.L., YANG Y., MUSHOTZKY R.F.
	Astrophys. J., 703, 2160-2170 (2009)
	The OPTX project. III. X-ray versus optical spectral type for active galactic nuclei.
o	Table 2: <CLANS NNN> (Nos 762-789) added.
=E=	Catalogue in electronic form as J/ApJS/179/1
=E=	Catalogue in electronic form as <J/ApJ/703/2160/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CLASC
CLASC	(COBRaS L-band All Source Catalogue)
Write:	<<CLASC NNa>>
N:	61+19
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	e-MERLIN L-band (21cm) observations of N=61+29 sources in the massive Cygnus OB2 association, as part of the COBRaS L-band All Source Catalogue (CLASC).
in source:	NAME VI Cyg = Ass Cyg OB 2
Ref:	=2020A&A...637A..64M
by	MORFORD J.C. , FENECH D.M., PRINJA R.K., BLOMME R., YATES J.A., DRAKE J.J., EYRES S.P.S., RICHARDS A.M.S., STEVENS I.R., WRIGHT N.J., CLARK J.S., DOUGHERTY S., PITTARD J.M., SMITH H.A., VINK J.S.
	Astron. Astrophys., 637A, 64-64 (2020)
	COBRaS: The e-MERLIN 21 cm Legacy survey of Cygnus OB2.
o	Fig. 5, Tables A.1-A.3: <CLASC NNa> N=61+19 among (Nos 1-61).
=E=	Catalogue in electronic form as <J/A+A/637/A64/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CLASH
CLASH	(Cluster Lensing And Supernova survey with Hubble)
Write:	<<CLASH {Abell\|A}NNNN NNNN>> <<CLASH RXJHHMM+DDMM NNNN>> <<CLASH MSHHMM+DDMM NNNN>> <<CLASH MACSJHHMM.m+DDMM NNNN>>
Object:	G (SIMBAD class: Galaxy)
Note:	HST ACS and WFC3 survey of 25 galaxy clusters. The Cluster Lensing And Supernova survey with Hubble (CLASH) overview paper is available at: Postman et al. 2012ApJS..199...25P. For more information, visit: http://www.stsci.edu/~postman/CLASH Data are available through the MAST archive: http://archive.stsci.edu/prepds/clash/
in source:	ACO 383
in source:	ACO 209
in source:	ACO 1423
in source:	ACO 2261
in source:	ClG J2129+0005 = RX J2129.6+0005
in source:	ACO 611
in source:	ClG 2137-2353 = 1E 2137.3-2353
in source:	ClG J1532+3021 = MCS J1532.9+3021
in source:	RX J2248.8+0937
in source:	ClG J1931-2635 = MCS J1931.8-2635
in source:	MCS J1115.8+0129
in source:	MCS J1720.2+3536
in source:	ClG J0429-0253 = MCS J0429.6-0253
in source:	MCS J0416.1-2403
in source:	MCS J1206.2-0847
in source:	ClG J0329-0212 = MCS J0329.7-0212
in source:	ClG J1347-1145 = RX J1347.5-1145
in source:	ClG J1311-0311 = MCS J1311.0-0311
in source:	ClG J1149+2223 = MCS J1149.5+2223
in source:	MCS J1423.8+2404
in source:	ClG J0717+3745 = MCS J0717.5+3745
in source:	ClG J2129-0741 = MCS J2129.4-0741
in source:	MCS J0647.0+7015
in source:	ClG J0744+3927 = MCS J0744.9+3927
in source:	ClG J1226+3332
Ref:	=2012ApJS..199...25P
by	POSTMAN M. , COE D., BENITEZ N., BRADLEY L., BROADHURST T., DONAHUE M., FORD H., GRAUR O., GRAVES G., JOUVEL S., KOEKEMOER A., LEMZE D., MEDEZINSKI E., MOLINO A., MOUSTAKAS L., OGAZ S., RIESS A., RODNEY S., ROSATI P., UMETSU K., ZHENG W., ZITRIN A., BARTELMANN M., BOUWENS R., CZAKON N., GOLWALA S., HOST O., INFANTE L., JHA S., JIMENEZ-TEJA Y., KELSON D., LAHAV O., LAZKOZ R., MAOZ D., McCULLY C., MELCHIOR P., MENEGHETTI M., MERTEN J., MOUSTAKAS J., NONINO M., PATEL B., REGOS E., SAYERS J., SEITZ S., VAN DER WEL A.
	Astrophys. J., Suppl. Ser., 199, 25 (2012)
	The Cluster Lensing And Supernova survey with Hubble: an overview.
o	Table 7: <CLASH MACS J1149.6+2223 NNNN> N=4629 among (Nos 1-9664).
Ref:	=2014A&A...562A..86J
by	JOUVEL S. , HOST O., LAHAV O., SEITZ S., MOLINO A., COE D., POSTMAN M., MOUSTAKAS L., BENITEZ N., ROSATI P., BALESTRA I., GRILLO C., BRADLEY L., FRITZ A., KELSON D., KOEKEMOER A.M., LEMZE D., MEDEZINSKI E., MERCURIO A., MOUSTAKAS J., NONINO M., SCODEGGIO M., ZHENG W., ZITRIN A., BARTELMANN M., BOUWENS R., BROADHURST T., DONAHUE M., FORD H., GRAVES G., INFANTE L., JIMENEZ-TEJA Y., LAZKOZ R., MELCHIOR P., MENEGHETTI M., MERTEN J., OGAZ S., UMETSU K.
	Astron. Astrophys., 562A, 86-86 (2014)
	CLASH: Photometric redshifts with 16 HST bands in galaxy cluster fields.
o	<CLASH MACS J1206.2-0847 NNNN> N=3510 among (Nos 6-6712).
=E=	Catalogue in electronic form as J/ApJS/199/25
=E=	Catalogue in electronic form as J/A+A/562/A86
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CLASHVLT
CLASHVLT	(Cluster Lensing And Supernova survey with Hubble - VLT)
Write:	<<CLASHVLT JHHMMSS.s+DDMMSS>> <<CLASHVLT JHHMMSS.ss+DDMMSS.s>>
N:	4386+4594+2653+283+280+2736
Object:	G (SIMBAD class: Galaxy)
Note:	VLT VIMOS spectroscopy of galaxies in the field of Frontier Fields galaxy clusters as part of the CLASH-VLT survey. For more information, visit: https://sites.google.com/site/vltclashpublic/home
in source:	MCS J0416.1-2403
in source:	ACO 209
in source:	ClG J2129-0741 = MCS J2129.4-0741
in source:	RXC J2248.7-4431 = ACO S 1063
in source:	MCS J1206.2-0847
Ref:	=2016ApJS..224...33B
by	BALESTRA I. , MERCURIO A., SARTORIS B., GIRARDI M., GRILLO C., NONINO M., ROSATI P., BIVIANO A., ETTORI S., FORMAN W., JONES C., KOEKEMOER A., MEDEZINSKI E., MERTEN J., OGREAN G.A., TOZZI P., UMETSU K., VANZELLA E., VAN WEEREN R.J., ZITRIN A., ANNUNZIATELLA M., CAMINHA G.B., BROADHURST T., COE D., DONAHUE M., FRITZ A., FRYE B., KELSON D., LOMBARDI M., MAIER C., MENEGHETTI M., MONNA A., POSTMAN M., SCODEGGIO M., SEITZ S., ZIEGLER B.
	Astrophys. J., Suppl. Ser., 224, 33-33 (2016)
	CLASH-VLT: dissecting the frontier fields galaxy cluster MACS J0416.1-2403 with ~800 spectra of member galaxies.
o	<CLASHVLT JHHMMSS.s+DDMMSS> N=4386.
Ref:	=2016A&A...585A.160A
by	ANNUNZIATELLA M. , MERCURIO A., BIVIANO A., GIRARDI M., NONINO M., BALESTRA I., ROSATI P., BARTOSCH CAMINHA G., BRESCIA M., GOBAT R., GRILLO C., LOMBARDI M., SARTORIS B., DE LUCIA G., DEMARCO R., FRYE B., FRITZ A., MOUSTAKAS J., SCODEGGIO M., KUCHNER U., MAIER C., ZIEGLER B.
	Astron. Astrophys., 585A, 160-160 (2016)
	CLASH-VLT: Environment-driven evolution of galaxies in the z = 0.209 cluster Abell 209.
o	<CLASHVLT JHHMMSS.ss+DDMMSS.s> N=2653.
Ref:	=2017MNRAS.466.4094M
by	MONNA A. , SEITZ S., BALESTRA I., ROSATI P., GRILLO C., HALKOLA A., SUYU S.H., COE D., CAMINHA G.B., FRYE B., KOEKEMOER A., MERCURIO A., NONINO M., POSTMAN M., ZITRIN A.
	Mon. Not. R. Astron. Soc., 466, 4094-4106 (2017)
	Precise strong lensing mass profile of the CLASH galaxy cluster MACS 2129.
o	<CLASHVLT JHHMMSS.ss+DDMMSS.s> N=283. Tables 2, A2: <[MSB2017b] NNNN> N=9+48 among (Nos 873-1676, 4248-17758), <[MSB2017b] BCG> N=1. Fig. 1: <[MSB2017b] GR> N=1, <[MSB2017b] GN> (Nos G1-G2). Figs 1+A2, Tables 3+A1: <[MSB2017b] NN> (Nos 1-22), <[MSB2017b] N.N> N=28 among (Nos 1.1-1.6 to 8.1-8.4), <[MSB2017b] N.Na> (Nos 4.1a-4.1b, 4.2a-4.2b, 4.3a-4.3b).
Ref:	=2017A&A...600A..90C
by	CAMINHA G.B. , GRILLO C., ROSATI P., BALESTRA I., MERCURIO A., VANZELLA E., BIVIANO A., CAPUTI K.I., DELGADO-CORREAL C., KARMAN W., LOMBARDI M., MENEGHETTI M., SARTORIS B., TOZZI P.
	Astron. Astrophys., 600A, 90-90 (2017)
	A refined mass distribution of the cluster MACS J0416.1-2403 from a new large set of spectroscopic multiply lensed sources.
o	Catalog: <CLASHVLT JHHMMSS.ss+DDMMSS.s> N=4594. Fig. 1, Table A.1: <[CGR2017b] MACS J0416 NNa> (Nos 1-37, 1a-1c to 37a-37c).
Ref:	=2017A&A...599A..28K
by	KARMAN W. , CAPUTI K.I., CAMINHA G.B., GRONKE M., GRILLO C., BALESTRA I., ROSATI P., VANZELLA E., COE D., DIJKSTRA M., KOEKEMOER A.M., McLEOD D., MERCURIO A., NONINO M.
	Astron. Astrophys., 599A, 28-28 (2017)
	MUSE integral-field spectroscopy towards the Frontier Fields cluster Abell S1063. II. Properties of low luminosity Lyman α emitters at z> 3.
o	Table A.1: <[KCC2017] NE-NNNa> N=120 among (Nos NE-1 to NE102b), <[KCG2015] NNa> N=12 among (Nos 68, 68a-68b, 69a-69b, 70, 70a-70b, 71-73, 77). Table B.1: <[MSG2014] NNNa> N=16 among (Nos 87a-87b to 100a-100b) added. <CLASHVLT JHHMMSS.ss+DDMMSS.s> N=280.
Ref:	=2013A&A...558A...1B
by	BIVIANO A. , ROSATI P., BALESTRA I., MERCURIO A., GIRARDI M., NONINO M., GRILLO C., SCODEGGIO M., LEMZE D., KELSON D., UMETSU K., POSTMAN M., ZITRIN A., CZOSKE O., ETTORI S., FRITZ A., LOMBARDI M., MAIER C., MEDEZINSKI E., MEI S., PRESOTTO V., STRAZZULLO V., TOZZI P., ZIEGLER B., ANNUNZIATELLA M., BARTELMANN M., BENITEZ N., BRADLEY L., BRESCIA M., BROADHURST T., COE D., DEMARCO R., DONAHUE M., FORD H., GOBAT R., GRAVES G., KOEKEMOER A., KUCHNER U., MELCHIOR P., MENEGHETTI M., MERTEN J., MOUSTAKAS L., MUNARI E., REGOS E., SARTORIS B., SEITZ S., ZHENG W.
	Astron. Astrophys., 558A, 1-1 (2013)
	CLASH-VLT: the mass, velocity-anisotropy, and pseudo-phase-space density profiles of the z = 0.44 galaxy cluster MACS J1206.2-0847.
o	<CLASHVLT JHHMMSS.s+DDMMSS> N=2736.
=E=	Catalogue in electronic form as <J/ApJS/224/33/>
=E=	Catalogue in electronic form as <J/A+A/600/A90/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CLASS
CLASS	(Cosmic Lens All-Sky Survey)
Write:	<<CLASS BHHMM+DDd>> <<CLASS JHHMMSS.ssss+DDMMSS.sss>>
N:	23418
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Cosmic Lens All-Sky Survey: Radio images of flat-spectrum radio sources to create a large sample of radio-loud gravitationally lensed systems. See the survey website: http://www.jb.man.ac.uk/research/gravlens/class/class.html 1996ApJ...473..595K: 1st ref. with objects of the CLASS survey.
Ref:	=1996ApJ...473..595K
by	KOCHANEK C.S.
	Astrophys. J., 473, 595-609 (1996)
	The flat-spectrum radio luminosity function, gravitational lensing, galaxy ellipticities, and cosmology.
o	MG 1131+045 = MITG J1131+0456
o	<CLASS BHHMM+DDd> N=2.
Ref:	=2003MNRAS.341....1M
by	MYERS S.T. , JACKSON N.J., BROWNE I.W.A., DE BRUYN A.G., PEARSON T.J., READHEAD A.C.S., WILKINSON P.N., BIGGS A.D., BLANDFORD R.D., FASSNACHT C.D., KOOPMANS L.V.E., MARLOW D.R., McKEAN J.P., NORBURY M.A., PHILLIPS P.M., RUSIN D., SHEPHERD M.C., SYKES C.M.
	Mon. Not. R. Astron. Soc., 341, 1-12 (2003)
	The Cosmic Lens All-Sky Survey - I. Source selection and observations.
o	Table 3: <CLASS JHHMMSS.ssss+DDMMSS.sss> N=23418.
=E=	Catalogue in electronic form as VIII/72
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CLASXS
CLASXS	(Chandra Large Area Synoptic X-ray Survey)
Write:	<<CLASXS NNN>>
N:	525
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	X-ray catalog from the Chandra Large Area Synoptic X-ray Survey (CLASXS). In ref. 2004AJ....128.1483S, photometry and finding charts for 521 of the 525 objects are given. A second designation with coordinate is also used by the authors, see CXCCLASXS.
in source:	NAME Lockman Hole Northwest Field
Ref:	=2004AJ....128.1501Y
by	YANG Y. , MUSHOTZKY R.F., STEFFEN A.T., BARGER A.J., COWIE L.L.
	Astron. J., 128, 1501-1523 (2004)
	The Chandra large area synoptic X-ray survey (CLASXS) of the Lockman Hole-northwest: the X-ray catalog.
o	Table 2, col(1): <CLASXS NNN> (Nos 1-525) = Table 2, col(2): <CXCCLASXS JHHMMSS.s+DDMMSS> N=525. Table 4: <[YMS2004] N> (Nos 1-4).
=E=	Catalogue in electronic form as J/AJ/128/1501
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CLB91]
[CLB91]	(Cristiani+La Franca+Barbieri+, 1991)
Write:	<<[CLB91] HHMMSS.s+DDMMSS>>
N:	52
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
in source:	SA 94-
Ref:	=1991MNRAS.250..531C
by	CRISTIANI S. , LA FRANCA F., BARBIERI C., CLOWES R.G., IOVINO A.
	Mon. Not. R. Astron. Soc., 250, 531-540 (1991)
	A complete quasar sample at intermediate redshift.
o	<Table 2: [CLB91] HHMMSS.s+DDMMSS> N=53
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLC2000]
[CLC2000]	(Contursi+Lequeux+Cesarsky+, 2000)
Write:	<<[CLC2000] peak A>>
N:	10
Object:	(Mid IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	ISOCAM observations. Map fig.5 of mid-IR emission peak in the region of LHA 115-N 66 in the SMC. See also [RCL2000].
in source:	Magellanic Clouds:SMC:LHA 115-N 66 = LHA 115-N 66
Ref:	=2000A&A...362..310C
by	CONTURSI A. , LEQUEUX J., CESARSKY D., BOULANGER F., RUBIO M., HANUS M., SAUVAGE M., TRAN D., BOSMA A., MADDEN S., VIGROUX L.
	Astron. Astrophys., 362, 310-324 (2000)
	Mid-infrared imaging and spectrophotometry of N66 in the SMC with ISOCAM.
o	Fig.5, note: object N-66-136, misprint for N-346-136 = Cl* NGC 346 MPG 136 in SIMBAD.
o	Fig.5: <[CLC2000] peak A> (Nos A-I).
Ref:	=2000A&A...359.1139R
by	RUBIO M. , CONTURSI A., LEQUEUX J., PROBST R., BARBA R., BOULANGER F., CESARSKY D., MAOLI R.
	Astron. Astrophys., 359, 1139-1146 (2000)
	Multiwavelength observations of N 66 in the SMC: unveiling photodissociation interfaces and star formation.
o	Table 1, Fig.8: <[CLC2000] peak A> (No. L) added. Fig.7: <[RCL2000] N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLC2016]
[CLC2016]	(Cunningham+Lumsden+Cyganowski+, 2016)
Write:	<<[CLC2016] SMAN>>
N:	4
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	SMA 1.3mm continuum observations towards NGC 2264-C.
in source:	NGC 2264C
Ref:	=2016MNRAS.458.1742C
by	CUNNINGHAM N. , LUMSDEN S.L., CYGANOWSKI C.J., MAUD L.T., PURCELL C.
	Mon. Not. R. Astron. Soc., 458, 1742-1767 (2016)
	Submillimeter array observations of NGC 2264-C: molecular outflows and driving sources.
o	Table 1: <[CLC2016] SMAN> (Nos 1-4).
o	© 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLC98]
[CLC98]	(Cernicharo+Lefloch+Cox+, 1998)= (TC) = (Trifid)
Write:	<<[CLC98] TCNNa>> <<[CLC98] A>>
N:	34+2
Object:	Condensation (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=17'Trifid Condensations' (TC in the format), and components or smaller ones. N=1 Jet 'J' and N=1 Bow-shock 'B'
in source:	NAME Trifid Nebula
Ref:	=1998Sci...282..462C
by	CERNICHARO J. , LEFLOCH B., COX P., CESARSKY D., ESTEBAN C., YUSEF-ZADEH F., MENDEZ D.I., ACOSTA-PULIDO J., GARCIA LOPEZ R.J., HERAS A.
	Science, 282, 462-465 (1998)
	Induced massive star formation in the Trifid nebula?
o	<HH NNN> (No. 399). Table 1: <[CLC98] TCN> (Nos TC0-TC4). Fig.3: <[CLC98] B>, <[CLC98] J>, N=2.
Ref:	=2000ApJ...545..340L
by	LEFLOCH B. , CERNICHARO J.
	Astrophys. J., 545, 340-352 (2000)
	Pre-Orion cores in the Trifid nebula.
o	Table 1: <[CLC98] TCNa> (Nos TC4b, TC4c) added.
Ref:	=2008A&A...489..157L
by	LEFLOCH B. , CERNICHARO J., PARDO J.R.
	Astron. Astrophys., 489, 157-171 (2008)
	Star formation in the Trifid Nebula. Cores and filaments.
o	Paragraph. 2.1 HD 164429A is a misprint for HD 164492A.
o	Fig.1, Table 2: <[LCP2008] WF> N=1, <[LCP2008] WL> (Nos EL, WL, SL). Fig.1, Table 3: <[CLC98] TCNNa> (Nos TC00, TC0a-TC0d, TC3a-TC3c,TC 4a, TC4f, TC5-TC17, TC6a-TC6d)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLD2007]
[CLD2007]	(Chu+Li+Desroches+, 2007)
Write:	<<[CLD2007] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	LOSS discovery of new SN. Host galaxy of SN 2007FR.
Ref:	=2007CBET.1001....1C
by	CHU J. , LI W.
	CBET, 1001, 1 (2007)
	Supernovae 2007fo, 2007fq, and 2007fr.
o	<[CLD2007] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLF2011]
[CLF2011]	(Cucchiara+Levan+Fow+, 2011)
Write:	<<[CLF2011] A>>
N:	3
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	UKIRT WFCAM and ESO 2.2m telescope GROND observations of the field of GRB 090429B.
Ref:	=2011ApJ...736....7C
by	CUCCHIARA A. , LEVAN A.J., FOX D.B., TANVIR N.R., UKWATTA T.N., BERGER E., KRUHLER T., KUPCU YOLDAS A., WU X.F., TOMA K., GREINER J., OLIVARES F.E., ROWLINSON A., AMATI L., SAKAMOTO T., ROTH K., STEPHENS A., FRITZ A., FYNBO J.P.U., HJORTH J., MALESANI D., JAKOBSSON P., WIERSEMA K., O'BRIEN P.T., SODERBERG A.M., FOLEY R.J., FRUCHTER A.S., RHOADS J., RUTLEDGE R.E., SCHMIDT B.P., DOPITA M.A., PODSIADLOWSKI P., WILLINGALE R., WOLF C., KULKARNI S.R., D'AVANZO P.
	Astrophys. J., 736, 7 (2011)
	A photometric redshift of z ~ 9.4 for GRB 090429B.
o	Fig. 4: the elliptical galaxy G1 is 2MASX J14024224+3210505 in SIMBAD.
o	Fig. 4, Table 4: <[CLF2011] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLF2014]
[CLF2014]	(Contreras Pena+Lucas+Froebrich+, 2014)= (GPSV) (Not yet in Simbad)
Write:	<<[CLF2014] GPSVNN>>
N:	45
Object:	V*
Note:	N=45 variable stars with ΔK>1mag. Use of the widely separated two-epoch K-band photometry in UKIDSS Galactic Plane Survey (UGPS) DR5 and DR7.
Ref:	=2014MNRAS.439.1829C
by	CONTRERAS PENA C. , LUCAS P.W., FROEBRICH D., KUMAR M.S.N., GOLDSTEIN J., DREW J.E., ADAMSON A., DAVIS C.J., BARENTSEN G., WRIGHT N.J.
	Mon. Not. R. Astron. Soc., 439, 1829-1854 (2014)
	Extreme infrared variables from UKIDSS - I. A concentration in star-forming regions.
o	Table 1: <[CLF2014] GPSVNN> (Nos GPSV1-GPSV45).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLF2019]
[CLF2019]	(Cheng+Li+Fang+, 2019) (Not yet in Simbad)
Write:	<<[CLF2019] NNN>>
N:	489
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	N=489 X-ray point sources in the massive globular cluster Terzan 5. Use of archival Chandra data. See also [CLL2019], [CML2020], [CLW2020].
in source:	Cl Terzan 5
Ref:	=2019ApJ...883...90C
by	CHENG Z. , LI Z., FANG T., LI X., XU X.
	Astrophys. J., 883, 90-90 (2019)
	Exploring the mass segregation effect of X-ray sources in globular clusters. II. The case of Terzan 5.
o	Table 2: <[CLF2019] NNN> (Nos 1-489).
=E=	Catalogue in electronic form as <J/ApJ/883/90/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLF98]
[CLF98]	(Courbin+Lidman+Frye+, 1998)
Write:	<<[CLF98] M Star>> <<[CLF98] Object E>>
N:	1+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Fig.3: 'Star M' and 'Object E' in the field of the PKS 1830-211. See also [SNP90] and [LFK2000].
Ref:	=1998ApJ...499L.119C
by	COURBIN F. , LIDMAN C., FRYE B.L., MAGAIN P., BROADHURST T.J., PAHRE M.A., DJORGOVSKI S.G.
	Astrophys. J., 499, 119-124 (1998)
	Image deconvolution of the radio ring PKS 1830-211.
o	Components NE and SW = [SNP90] 1830-211 NE and SW.
o	Fig.3: <[CLF98] M Star> N=1, <[CLF98] Object E> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ClG
ClG	(Cluster of G)= (C) = (Cl)
Write:	<<ClG HHMM+DD>> <<ClG HHMM.m+DD>> <<ClG HHMM+DDMM>> <<ClG HHMM.m+DDMM>> <<ClG JHHMM+DDMM>> <<ClG JHHMM.m+DDMM>>
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	Systematic Designation
Details on Acronym: [CLG2006]
[CLG2006]	(Carrasco-Gonzalez+Lopez+Gyulbudaghian+, 2006)
Write:	<<[CLG2006] N>>
N:	8
Object:	Dark Globule (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	Halpha imaging at the IAC-80 telescope. New radial system of dark globules associated with LBN 978 HII region.
in source:	LBN 978
Ref:	=2006A&A...445L..43C
by	CARRASCO-GONZALEZ C. , LOPEZ R., GYULBUDAGHIAN A., ANGLADA G., LEE C.W.
	Astron. Astrophys., 445, 43-46 (2006)
	A new radial system of dark globules in Monoceros.
o	Table 2: <[CLG2006] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLG2011]
[CLG2011]	(Carretta+Lucatello+Gratton+, 2011)
Write:	<<[CLG2011] NNNNN>>
N:	124
Object:	RGB* (SIMBAD class: RGB* = Red Giant Branch star)
Note:	VLT FLAMES observations of N=124 red giant stars in NGC 1851.
in source:	NGC 1851
Ref:	=2011A&A...533A..69C
by	CARRETTA E. , LUCATELLO S., GRATTON R.G., BRAGAGLIA A., D'ORAZI V.
	Astron. Astrophys., 533A, 69-69 (2011)
	Multiple stellar populations in the globular cluster NGC 1851.
o	Tables 2-8: <[CLG2011] NNNNN> N=124 among (Nos 13618-53106).
=E=	Catalogue in electronic form as J/A+A/533/A69
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLG2020]
[CLG2020]	(Cassata+Liu+Groves+, 2020)
Write:	<<[CLG2020] GalN>>
N:	5
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 3 and Band 4 observations of N=5 star-forming galaxies at 3<z<3.5.
Ref:	=2020ApJ...891...83C
by	CASSATA P. , LIU D., GROVES B., SCHINNERER E., IBAR E., SARGENT M., KARIM A., TALIA M., LE FEVRE O., TASCA L., LEMAUX B.C., RIBEIRO B., FIORE S., ROMANO M., MANCINI C., MORSELLI L., RODIGHIERO G., RODRIGUEZ-MUNOZ L., ENIA A., SMOLCIC V.
	Astrophys. J., 891, 83-83 (2020)
	ALMA reveals the molecular gas properties of five star-forming galaxies across the main sequence at 3.
o	Fig. 2, Table 1: <[CLG2020] GalN> (Nos Gal1-Gal5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLG99]
[CLG99]	(Covino+Lazzati+Ghisellini+, 1999)
Write:	<<[CLG99] A>>
N:	3
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=3 stars in the field of GRB 990510, (Nos A-C), identical to [BHR99] A to C. See also [BHR99] and [PU99].
Ref:	=1999A&A...348L...1C
by	COVINO S. , LAZZATI D., GHISELLINI G., SARACCO P., CAMPANA S., CHINCARINI G., DI SEREGO S., CIMATTI A., VANZI L., PASQUINI L., HAARDT F., ISRAEL G.L., STELLA L., VIETRI M.
	Astron. Astrophys., 348, 1-4 (1999)
	GRB 990510: linearly polarized radiation from a fireball.
o	(Erratum) Erratum vol. 351, p. 399 (1999)
o	Fig.1: <[CLG99] A> (Nos A-B).
Ref:	=1999A&A...348L...5I
by	ISRAEL G.L. , MARCONI G., COVINO S., LAZZATI D., GHISELLINI G., CAMPANA S., GUZZO L., GUERRERO G., STELLA L.
	Astron. Astrophys., 348, 5-8 (1999)
	ESO deep observations of the optical afterglow of GRB 990510.
o	Fig.1: <[CLG99] A> (No. C) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLH2000]
[CLH2000]	(Cox+Lucas+Huggins+, 2000) (Not yet in Simbad)
Write:	<<[CLH2000] AN>>
N:	12
Object:	Outflow (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=6 pairs of opposite direction CO outflows (Nos A1-A2 to G1-G2). See also [SHK98].
in source:	RAFGL 2688
Ref:	=2000A&A...353L..25C
by	COX P. , LUCAS R., HUGGINS P.J., FORVEILLE T., BACHILLER R., GUILLOTEAU S., MAILLARD J.P., OMONT A.
	Astron. Astrophys., 353, 25-28 (2000)
	Multiple molecular outflows in AFGL 2688.
o	Fig.3: <[CLH2000] AN> (Nos A1-A2 to G1-G2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLH2009]
[CLH2009]	(Chynoweth+Langston+Holley-Bockelmann+, 2009)
Write:	<<[CLH2009] N>> <<[CLH2009] C09-N>> (not recognised by Simbad, but found in literature)
N:	3
Object:	HI Cloud (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	GBT HI observations of the NGC 2403 group. See also [CLY2008], [CLH2011].
in source:	NAME NGC 2403 GROUP
Ref:	=2009AJ....138..287C
by	CHYNOWETH K.M. , LANGSTON G.I., HOLLEY-BOCKELMANN K., LOCKMAN F.J.
	Astron. J., 138, 287-294 (2009)
	A search for diffuse neutral hydrogen and H I clouds in the NGC 2403 group.
o	Table 5: <[CLH2009] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLH2011]
[CLH2011]	(Chynoweth+Langston+Holley-Bockelmann, 2011)= ([CLH2011a])
Write:	<<[CLH2011] N>> <<[CLH2011] C10-N>> (not recognised by Simbad, but found in literature)
N:	5
Object:	HI Cloud (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	GBT HI observations of the M81 filament. See also [CLY2008], [CLH2009].
Ref:	=2011AJ....141....9C
by	CHYNOWETH K.M. , LANGSTON G.I., HOLLEY-BOCKELMANN K.
	Astron. J., 141, 9 (2011)
	H I clouds in the M81 filament as dark matter minihalos–a phase-space mismatch.
o	Table 1, col(1): <[CLH2011] N> (Nos 1-5). Table 1, col(2): <GBC JHHMMSS.s+DDMMSS> N=13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
History	of this Acronym: replaced by GBC (for format JHHMMSS.s+DDMMSS)
Details on Acronym: [CLH2011]
[CLH2011]	(Chynoweth+Langston+Holley-Bockelmann, 2011)
*****	Avoid the usage of [CLH2011], prefer GBC
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLH2011a]
[CLH2011a]	(Chynoweth+Langston+Holley-Bockelmann, 2011)
*****	Avoid the usage of [CLH2011a], prefer [CLH2011]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
History	of this Acronym: replaced by GBC (for format JHHMMSS.s+DDMMSS)
Details on Acronym: [CLH2011b]
[CLH2011b]	(Clem+Landolt+Hoard+, 2011)
Write:	<<[CLH2011b] NNNNNN>>
N:	316367
Object:	* (SIMBAD class: Star)
Note:	CTIO 0.9m telescope photometric observations of N=316367 stars in the open cluster NGC 3532. Use of archival 2MASS data.
in source:	NGC 3532
Ref:	=2011AJ....141..115C
by	CLEM J.L. , LANDOLT A.U., HOARD D.W., WACHTER S.
	Astron. J., 141, 115 (2011)
	Deep, wide-field CCD photometry for the open cluster NGC 3532.
o	Table 2: <[CLH2011b] NNNNNN> (Nos 1-316367).
=E=	Catalogue in electronic form as <J/AJ/141/115/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLH2012]
[CLH2012]	(Cantalupo+Lilly+Haehnelt+, 2012)
Write:	<<[CLH2012] NNNN>> <<[CLH2012] LAB1>>
N:	98
Object:	LAE + Blob-like extended emitter (SIMBAD class: EmObj = Emission Object)
Note:	VLT FORS observations of N=98 Lyman α candidates and N=1 blob-like extended emission in a large cosmological volume centred on the hyperluminous z=2.4 quasar HE 0109-3518.
Ref:	=2012MNRAS.425.1992C
by	CANTALUPO S. , LILLY S.J., HAEHNELT M.G.
	Mon. Not. R. Astron. Soc., 425, 1992-2014 (2012)
	Detection of dark galaxies and circum-galactic filaments fluorescently illuminated by a quasar at z = 2.4.
o	Tables 2-3, A1: <[CLH2012] NNNN> N=31+7+60 among (Nos 90-2985). Paragr. 3: <[CLH2012] LAB1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLJ2019]
[CLJ2019]	(Coutens +Liu+Jimenez-Serra+, 2019)
Write:	<<[CLJ2019] JHHMMSS.ss+DDMMSS.s>>
N:	42
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	JVLA 10GHz observations of N=42 YSO candidates in the Oph A star-forming region.
in source:	NAME rho Oph A
Ref:	=2019A&A...631A..58C
by	COUTENS A. , LIU H.B., JIMENEZ-SERRA I., BOURKE T.L., FORBRICH J., HOARE M., LOINARD L., TESTI L., AUDARD M., CASELLI P., CHACON-TANARRO A., CODELLA C., DI FRANCESCO J., FONTANI F., HOGERHEIJDE M., JOHANSEN A., JOHNSTONE D., MADDISON S., PANIC O., PEREZ L.M., PODIO L., PUNANOVA A., RAWLINGS J.M.C., SEMENOV D., TAZZARI M., TOBIN J.J., VAN DER WIEL M.H.D., VAN LANGEVELDE H.J., VLEMMINGS W., WALSH C., WILNER D.
	Astron. Astrophys., 631A, 58-58 (2019)
	VLA cm-wave survey of young stellar objects in the Oph A cluster: constraining extreme UV- and X-ray-driven disk photoevaporation. A pathfinder for Square Kilometre Array studies.
o	Table B.1: <[CLJ2019] JHHMMSS.ss+DDMMSS.s> N=42.
=E=	Catalogue in electronic form as <J/A+A/631/A58/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLK2012]
[CLK2012]	(Chies-Santos+Larsen+Kissler-Patig, 2012)
Write:	<<[CLK2012] NN>>
N:	23
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	VLT FORS2 spectroscopy of N=23 globular cluster candidates in the Virgo Cluster elliptical NGC 4365.
in source:	NGC 4365
Ref:	=2012MNRAS.427.2349C
by	CHIES-SANTOS A.L. , LARSEN S.S., KISSLER-PATIG M.
	Mon. Not. R. Astron. Soc., 427, 2349-2358 (2012)
	The old globular cluster system of NGC4365: new VLT/FORS2 spectra.
o	Fig. 1, Table 1: <[CLK2012] NN> N=23 among (Nos 07-29).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLK2019]
[CLK2019]	(Chung+Lee+Kim+, 2019)
Write:	<<[CLK2019] FNN>> <<[CLK2019] FN-CN>>
N:	10+8
Object:	C18O Filament + N2H+ Core (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	TRAO 14m telescope observations of N=10 C18O filaments and N=8 N2H+ dense cores in LDN 1478, the central region of the California Molecular Cloud, as part of the TRAO FUNS project. See also [CLK2021].
in source:	LDN 1478
Ref:	=2019ApJ...877..114C
by	CHUNG E.J. , LEE C.W., KIM S., KIM G., CASELLI P., TAFALLA M., MYERS P.C., SOAM A., LIU T., GOPINATHAN M., KIM M., KIM K.H., KWON W., KANG H., LEE C.
	Astrophys. J., 877, 114-114 (2019)
	TRAO survey of nearby filamentary molecular clouds, the universal nursery of stars (TRAO FUNS). I. Dynamics and chemistry of L1478 in the California molecular cloud.
o	Fig. 3, Table 3: <[CLK2019] FNN> (Nos F1-F10). Figs 4-5, Table 2: <[CLK2019] FN-CN> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLK2021]
[CLK2021]	(Chung+Lee+Kim+, 2021)
Write:	<<[CLK2021] FNNa>> <<[CLK2021] CNN>> <<[CLK2021] CLNN>>
N:	24+22+30
Object:	C18O Filament + N2H+ Core + C18O Clump (SIMBAD class: Unknown = Object of Unknown Nature)
Stat.	in SIMBAD: Tables 3 et 6 completes
Note:	TRAO 14m telescope observations of N=24 C18O filaments, N=22 N2H+ dense cores, and N=30 C18O clumps in the field of IC 5146, as part of the TRAO FUNS project. See also [CLK2019].
in source:	IC 5146
Ref:	=2021ApJ...919....3C
by	CHUNG E.J. , LEE C.W., KIM S., GOPINATHAN M., TAFALLA M., CASELLI P., MYERS P.C., LIU T., YOO H., KIM K.H., KIM M.-R., SOAM A., CHO J., KWON W., LEE C., KANG H.
	Astrophys. J., 919, 3-3 (2021)
	TRAO survey of the nearby filamentary molecular clouds, the universal nursery of stars (TRAO FUNS). II. Filaments and dense cores in IC 5146.
o	Fig. 4, Table 2: <[CLK2021] FNNa> (Nos F1, F1a-F1b, F2-4, F4a-F4h, F5-F6, F6a-F6b, F7-F9, F9a-F9b, F10-F14). Fig. 9, Table 3: <[CLK2021] CNN> (Nos C1-C22).Table 6: <[CLK2021] CLNN> (Nos CL1-CL30).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLK98]
[CLK98]	(Clowe+Luppino+Kaiser+, 1998) (Not yet in Simbad)
Write:	<<[CLK98] A>>
N:	5
Object:	Arc (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Observation of the ClG 1E 1137.5+6625. Fig.1: (Nos A-B) are 2 giant arcs, No. C is a counterarc candidate, (Nos C-D) are 2 giant arc candidates.
in source:	1E 1137.0+6625
Ref:	=1998ApJ...497L..61C
by	CLOWE D. , LUPPINO G.A., KAISER N., HENRY J.P., GIOIA I.M.
	Astrophys. J., 497, 61-64 (1998)
	Weak lensing by two z~0.8 clusters of galaxies.
o	ClG MS 1137+66 = 1E 1137.5+6625, RX J1716+67 = RX J1716.6+6708, MS 1054-03 = 1E 1054.5-0321
o	Fig.1: <[CLK98] A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLL2019]
[CLL2019]	(Cheng+Li+Li+, 2019) (Not yet in Simbad)
Write:	<<[CLL2019] NNN>>
N:	537
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	N=537 X-ray sources in the globular cluster 47 Tuc. Use of archival Chandra data. See also [CLF2019], [CML2020], [CLW2020].
in source:	NGC 104 = 47 Tuc
Ref:	=2019ApJ...876...59C
by	CHENG Z. , LI Z., LI X., XU X., FANG T.
	Astrophys. J., 876, 59-59 (2019)
	Exploring the mass segregation effect of X-ray sources in globular clusters: the case of 47 Tucanae.
o	Table 2, col(1): <[CLL2019] NNN> (Nos 1-537).
=E=	Catalogue in electronic form as <J/ApJ/876/59/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLM2001]
[CLM2001]	(Carson+Larkin+McLean+, 2001) (Not yet in Simbad)
Write:	<<[CLM2001] 4C 48.48 CN>>
N:	5
Object:	Component (SIMBAD class: PartofG = Part of a Galaxy)
Note:	N=5 components of the radio galaxy 4C 48.48.
in source:	4C 48.48
Ref:	=2001ApJ...563...63C
by	CARSON J.E. , LARKIN J.E., McLEAN I.S., GRAHAM J.R., BECKLIN E.E., FIGER D.F., GILBERT A.M., LEVENSON N.A., TEPLITZ H.I., WILCOX M.K.
	Astrophys. J., 563, 63-70 (2001)
	Resolved infrared spectroscopy of two high-redshift radio galaxies.
o	Fig.1, Table 2: <[CLM2001] 4C 48.48 CN> (Nos C1-C5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLM2002]
[CLM2002]	(Courbin+Letawe+Magain+, 2002)
Write:	<<[CLM2002] GN>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ESO NTT observations. One galaxy in the field of HE 1503+0228, unrelated to the QSO.
Ref:	=2002A&A...394..863C
by	COURBIN F. , LETAWE G., MAGAIN P., WISOTZKI L., JABLONKA P., JAHNKE K., KUHLBRODT B., ALLOIN D., MEYLAN G., MINNITI D., BURUD I.
	Astron. Astrophys., 394, 863-872 (2002)
	On-axis spatially resolved spectroscopy of low redshift quasar host galaxies: HE 1503+0228, at z=0.135.
o	Fig. 1 : PSF = USNO-A2.0 0900-07894800
o	Fig.1: <[CLM2002] GN> (No. G1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLM2003]
[CLM2003]	(Cuby+Le Fevre+McCracken+, 2003)= ([CLM2003a])
Write:	<<[CLM2003] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	CFHT and VLT observations. Discovery of a galaxy with z = 6.17.
Ref:	=2003A&A...405L..19C
by	CUBY J.-G. , LE FEVRE O., McCRACKEN H., CUILLANDRE J.-C., MAGNIER E., MENEUX B.
	Astron. Astrophys., 405, 19-22 (2003)
	Discovery of a z = 6.17 galaxy from CFHT and VLT observations.
o	Table 1: <[CLM2003] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLM2003a]
[CLM2003a]	(Cuby+Le Fevre+McCracken+, 2003)
*****	Avoid the usage of [CLM2003a], prefer [CLM2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLM2003b]
[CLM2003b]	(Chen+Lu+Mendez+, 2003)
Write:	<<[CLM2003b] xxxyyNNNA>>
N:	2615
Object:	* (SIMBAD class: Star)
Note:	CTIO and KPNO observations. Spectrophotometry of 2615 stars in the SGP. In the format xxx stands for the field pixel number in decreasing RA, yy the field pixel number in increasing Dec, NNN a serial number in the field, the letter A for binary components.
in source:	NAME SGP
Ref:	=2003AJ....126..762C
by	CHEN A.B.-C. , LU P.K., MENDEZ R.A., VAN ALTENA W.F.
	Astron. J., 126, 762-771 (2003)
	Dark matter: local volume density versus total surface density.
o	Catalogue: <[CLM2003b] xxxyyNNNA> N=2615.
=E=	Catalogue in electronic form as J/AJ/126/762
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLM2007]
[CLM2007]	(Chapman+Lai+Mundy+, 2007)= (OC) (Not yet in Simbad)
Write:	<<[CLM2007] Lupus OCN>>
Object:	Region (SIMBAD class: Region = Region defined in the Sky)
Note:	Spitzer Space Telescope MIPS observations of the Lupus Cloud. N=2 'Off-Cloud' regions.
in source:	NAME Lupus Cloud
Ref:	=2007ApJ...667..288C
by	CHAPMAN N.L. , LAI S.-P., MUNDY L.G., EVANS II N.J., BROOKE T.Y., CIEZA L.A., SPIESMAN W.J., REBULL L.M., STAPELFELDT K.R., NORIEGA-CRESPO A., LANZ L., ALLEN L.E., BLAKE G.A., BOURKE T.L., HARVEY P.M., HUARD T.L., JORGENSEN J.K., KOERNER D.W., MYERS P.C., PADGETT D.L., SARGENT A.I., TEUBEN P., VAN DISHOECK E.F., WAHHAJ Z., YOUNG K.E.
	Astrophys. J., 667, 288-302 (2007)
	The Spitzer c2d Survey of large, nearby, interstellar clouds. IV. Lupus observed with MIPS.
o	Fig.1, Table 1: <[CLM2007] Lupus OCN> (Nos OC1, OC2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLM2017]
[CLM2017]	(Contreras Pena+Lucas+Minniti+, 2017)= (VVVv)
Write:	<<[CLM2017] VVVvNNN>>
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	N=816 high-amplitude infrared variable stars (ΔK_s>1mg) in the VISTA Variables in the Via Lactea (VVV) survey.
Ref:	=2017MNRAS.465.3011C
by	CONTRERAS PENA C. , LUCAS P.W., MINNITI D., KURTEV R., STIMSON W., NAVARRO MOLINA C., BORISSOVA J., KUMAR M.S.N., THOMPSON M.A., GLEDHILL T., TERZI R., FROEBRICH D., CARATTI O GARATTI A.
	Mon. Not. R. Astron. Soc., 465, 3011-3038 (2017)
	A population of eruptive variable protostars in VVV.
o	Table 2, col(1): <[CLM2017] VVVvNNN> (Nos VVVv1-VVVv816).
=E=	Catalogue in electronic form as <J/MNRAS/465/3011/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLM98]
[CLM98]	(Courbin+Lidman+Magain, 1998)
Write:	<<[CLM98] GN>> <<[CLM98] Star N>>
N:	2+3
Object:	G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=2 galaxies (Nos G1-G2), and N=3 stars in the field of HE 1104-1805 Map in Fig.1
Ref:	=1998A&A...330...57C
by	COURBIN F. , LIDMAN C., MAGAIN P.
	Astron. Astrophys., 330, 57-62 (1998)
	Detection of the lensing galaxy in HE 1104-1805.
o	QSO A and B = [WKK93] HE 1104-1805 A and B
o	Fig.1: <[CLM98] GN> (Nos G1-G2), <[CLM98] Star N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CLN
CLN	(Cometary Like Nebula)
*****	Avoid the usage of CLN, prefer [G98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CLO2013]
[CLO2013]	(Cooper+Lumsden+Oudmaijer+, 2013)
Write:	<<[CLO2013] GLLL.llll+BB.bbbbA-N>>
N:	28
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	UKIRT UIST observations of YSO candidates selected from the MSX RMS survey.
Ref:	=2013MNRAS.430.1125C
by	COOPER H.D.B. , LUMSDEN S.L., OUDMAIJER R.D., HOARE M.G., CLARKE A.J., URQUHART J.S., MOTTRAM J.C., MOORE T.J.T., DAVIES B.
	Mon. Not. R. Astron. Soc., 430, 1125-1157 (2013)
	The RMS survey: near-IR spectroscopy of massive young stellar objects.
o	Tables A1-A3: <[CLO2013] GLLL.llll+BB.bbbbA-N> N=28.
=E=	Catalogue in electronic form as J/MNRAS/430/1125/sources
=E=	Catalogue in electronic form as <J/MNRAS/430/1125/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Cloud
Cloud	(Type of object) (Not yet in Simbad)
*****	Avoid the usage of Cloud, prefer [SS72]
Details on Acronym: Cloud
Cloud	(Type of object)
*****	Avoid the usage of Cloud, prefer [V69]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [CLP2003]
[CLP2003]	(Claria+Lapasset+Piatti+, 2003)
Write:	<<[CLP2003] NNN>>
N:	273
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	LCO and CTIO observations. UBV photoelectric photometry of stars in the fields of the 2 open clusters IC 2395 and Cl VDBH 47. The authors postulate that there is only one cluster IC 2395 = Cl VDBH 47.
in source:	IC 2395
in source:	Cl VDBH 47
Ref:	=2003A&A...409..541C
by	CLARIA J.J. , LAPASSET E., PIATTI A.E., AHUMADA A.V.
	Astron. Astrophys., 409, 541-551 (2003)
	IC2395 and BH47: Only one open cluster in the Vela constellation.
o	Table 1: <[CLP2003] NNN> (Nos 1-273).
=E=	Catalogue in electronic form as J/A+A/409/541
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLP2007]
[CLP2007]	(Cantalupo+Lilly+Porciani, 2007)
Write:	<<[CLP2007] NN>>
N:	13
Object:	LAE (SIMBAD class: EmObj = Emission Object)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 observations. Search for Lyman-alpha emitters around QSO 0420-388.
Ref:	=2007ApJ...657..135C
by	CANTALUPO S. , LILLY S.J., PORCIANI C.
	Astrophys. J., 657, 135-144 (2007)
	Plausible fluorescent Lyα emitters around the z = 3.1 QSO 0420-388.
o	Table 2: <[CLP2007] NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLP2009]
[CLP2009]	(Currie+Lada+Plavchan+, 2009)
Write:	<<[CLP2009] NNNN>> <<[CLP2009] DDD.dddd+DD.dddd>>
N:	8642+1143
Object:	* (SIMBAD class: Star)
Note:	Spitzer IRAC and MIPS observations of NGC 2362. Use of archival 2MASS data.
in source:	NGC 2362
Ref:	=2009ApJ...698....1C
by	CURRIE T. , LADA C.J., PLAVCHAN P., ROBITAILLE T.P., IRWIN J., KENYON S.J.
	Astrophys. J., 698, 1-27 (2009)
	The last gasp of gas giant planet formation: a Spitzer study of the 5 Myr old cluster NGC 2362.
o	Table 1: <[CLP2009] NNNN> (Nos 1-8642). Table 3: <[CLP2009] DDD.dddd+DD.dddd> N=1143.
=E=	Catalogue in electronic form as <J/ApJ/698/1/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLP99]
[CLP99]	(Chen+Lanzetta+Pascarelle, 1999)
Write:	<<[CLP99] Galaxy A>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	STIS observations on HST Observations of 'Galaxy A' at a probable redshift z=6.68, and its neighbours with another galaxy, 'Galaxy B'.
Ref:	=1999Natur.398..586C
by	CHEN H.-W. , LANZETTA K.M., PASCARELLE S.
	Nature, 398, 586-588 (1999)
	Spectroscopic identification of a galaxy at a probable redshift of z = 6.68.
o	<[CLP99] Galaxy A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLR2000]
[CLR2000]	(Claeskens+Lee+Remy+, 2000)
Write:	<<[CLR2000] GN>> <<[CLR2000] CSN>> <<[CLR2000] QSO 1548+114A A>> <<[CLR2000] NNN>>
N:	3+2+2+83
Object:	G + * (SIMBAD class: Galaxy)
Note:	ESO NTT and HST observations. Figs 1, 4: N=3 galaxies in the field of QSO 1548+114A, (Nos G1-G3), already observed without designations in 1974Natur.250..308S. Fig.1: N=2 Comparison Stars, (Nos CS1-CS2). Table 3: 'H' is the host galaxy of QSO 1548+114A, 'C' is a companion galaxy. Table 3: N=83 objects, format 'NNN' within 45" from QSO 1548+114A.
Ref:	=2000A&A...356..840C
by	CLAESKENS J.-F. , LEE D.-W., REMY M., SLUSE D., SURDEJ J.
	Astron. Astrophys., 356, 840-848 (2000)
	QSO mass constraints from gravitational lensing studies of quasar pairs. The cases of Q1548+114 A & B and Q1148+0055 A & B.
o	Figs 1, 4: <[CLR2000] GN> (Nos G1-G3). Fig.1: <[CLR2000] CSN> (Nos CS1-CS2). Table 3: <[CLR2000] QSO 1548+114A A> (Nos H, C), <[CLR2000] NNN> N=83 among 157.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLR2010]
[CLR2010]	(Covey+Lada+Roman-Zuniga+, 2010)
Write:	<<[CLR2010] NWW>>
N:	9+2
Object:	(NIR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Stat:	is completely incorporated in Simbad
Note:	IRTF SpeX spectroscopy of Spitzer MIPS bright sources.
in source:	Barnard 59
Ref:	=2010ApJ...722..971C
by	COVEY K.R. , LADA C.J., ROMAN-ZUNIGA C., MUENCH A.A., FORBRICH J., ASCENSO J.
	Astrophys. J., 722, 971-988 (2010)
	The age, stellar content, and star formation timescale of the B59 dense core.
o	Table 2: [BHB2007] 18SW, [CLR2010] 2 and [CLR2010] 2NE are not in SIMBAD (no coordinates).
o	Fig. 1, Table 2: <[CLR2010] NWW> (Nos 1-2, 2NE-2SW, 3-9). Fig. 2, Table 1: <[BHB2007] NNWW> (Nos 8NW-8SE, 13NW, 18NE-18SW).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CLS
CLS	(Case univ., Late *)
Write:	<<CLS NNNA>>
N:	132
Object:	Red * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	132 faint red stars that show definite or strongly suspected carbon or late M-type spectra. Red magnitudes ranging from 9 to 17, area with approximate boundaries 8h15m < alpha < 17h30m and +29deg < delta < +38deg Identif. charts
Ref:	=1988ApJS...66..387S
by	SANDULEAK N. , PESCH P.
	Astrophys. J., Suppl. Ser., 66, 387-390 (1988)
	The case low-dispersion northern sky survey. VII. Late-type stars.
o	(Erratum) Erratum 1996 ApJS 103, p. 513
o	Table 1: <CLS NNN-A> (Nos 1-122), N=132
=E=	Catalogue in electronic form as J/ApJS/66/387
Details on Acronym: [CLS2001]
[CLS2001]	(Chapman+Lewis+Scott+, 2001)= (SMM)
Write:	<<[CLS2001] SMM JHHMMSS+DDMM>>
N:	5
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SCUBA observations. N=5 submillimeter sources within the 2 blob regions [SAS2000] Blob 1 and 2. See [SAD98] and [SAS2000].
Ref:	=2001ApJ...548L..17C
by	CHAPMAN S.C. , LEWIS G.F., SCOTT D., RICHARDS E., BORYS C., STEIDEL C.C., ADELBERGER K.L., SHAPLEY A.E.
	Astrophys. J., 548, 17-21 (2001)
	Submillimeter imaging of a protocluster region at z=3.09.
o	Table 1: <[CLS2001] SMM JHHMMSS+DDMM> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLS2005]
[CLS2005]	(Cypriano+Lima Neto+Sodre+, 2005)
Write:	<<[CLS2005] CSSs-MMSS>> <<[CLS2005] GSSs-MMSS>>
N:	31+13
Object:	G in ClG + G (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Gemini North Telescope GMOS and Chandra observations of ACO 586: 31 galaxies members of the cluster + 13 noncluster member galaxies. In the format, the letter C stands for cluster member, the letter G for noncluster member, and the complete 2000 coordintes are 07 32 SSs +31 MM SS.
in source:	ACO 586
Ref:	=2005ApJ...630...38C
by	CYPRIANO E.S. , LIMA NETO G.B., SODRE L.Jr, KNEIB J.-P., CAMPUSANO L.E.
	Astrophys. J., 630, 38-49 (2005)
	Gemini and Chandra observations of Abell 586, a relaxed strong-lensing cluster.
o	Table 1: coordinates of [CLS2005] C107-3616 and C107-3725 are inverted. Table 2: coordinates of [CLS2005] G298-3552 and G298-3623 are inverted.
o	Table 1: <[CLS2005] CSSs-MMSS> N=31. Table 2: <[CLS2005] GSSs-MMSS> N=13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLT2003]
[CLT2003]	(Chandar+Leitherer+Tremonti+, 2003)
Write:	<<[CLT2003] Cluster N>>
N:	5
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST STIS observations. N=5 star clusters in Hen 2-10 galaxy.
in source:	Hen 2-10
Ref:	=2003ApJ...586..939C
by	CHANDAR R. , LEITHERER C., TREMONTI C., CALZETTI D.
	Astrophys. J., 586, 939-958 (2003)
	The stellar content of Henize 2-10 from Space Telescope Imaging Spectrograph ultraviolet spectroscopy.
o	Table 1: <[CLT2003] Cluster N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLT2004]
[CLT2004]	(Chandar+Leitherer+Tremonti, 2004)
Write:	<<[CLT2004] He 2-10 N>> <<[CLT2004] Mrk NNN N>> <<[CLT2004] NGC NNNN N>> <<[CLT2004] Tol 1924-416 N>> <<[CLT2004] Tol 89 N>>
N:	22
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST STIS ultraviolet spectroscopy of star clusters in local starburst galaxies.
in source:	Hen 2-10
in source:	Mrk 36
in source:	Mrk 209
in source:	NGC 1741
in source:	NGC 3049
in source:	NGC 3125
in source:	NGC 3310
in source:	NGC 4214
in source:	NGC 4670
in source:	NGC 5102
in source:	NGC 5996
in source:	NGC 6744
in source:	NGC 7552
in source:	Tol 1924-416
in source:	Tol 89
Ref:	=2004ApJ...604..153C
by	CHANDAR R. , LEITHERER C., TREMONTI C.A.
	Astrophys. J., 604, 153-166 (2004)
	NGC 3125-1: the most extreme Wolf-Rayet star cluster known in the local universe.
o	NGC 5253-5 = [CMB97] NGC 5253-5
o	Table 2: <[CLT2004] He 2-10 N> (No. 1), <[CLT2004] Mrk NNN N> N=2, <[CLT2004] NGC NNNN N> N=13, <[CLT2004] Tol 1924-416 N> (No. 1), <[CLT2004] Tol 89 N> (No. 1).
Ref:	=2005ApJ...628..210C
by	CHANDAR R. , LEITHERER C., TREMONTI C.A., CALZETTI D., ALOISI A., MEURER G.R., DE MELLO D.
	Astrophys. J., 628, 210-230 (2005)
	The stellar content of nearby star-forming galaxies. III. Unravelling the nature of the diffuse ultraviolet light.
o	Text: <[CLT2004] NGC 1741 N> (Nos 2-4) added, <[CLT2004] NGC 4670 N> (Nos 2-4) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CLU
CLU	(Census of the Local Universe)
Write:	<<CLU JHHMMSS.ss+DDMMSS.s>>
N:	about 269000000
Object:	Visual
Note:	The Census of the Local Universe (CLU) is a narrow-band survey that searches for emission-line (Halpha) galaxies across ∼3π of the sky (26,470deg²) with 4 narrow-band filters that probe a distance out to 200Mpc. The images are taken with a 7.92deg² mosaic imager composed of 12 CCD detectors with a 1 arcsec per pixel image scale on the Oschin 48inch telescope located atop Palomar observatory. The first filter is centered near the z=0 Hα emission line (lambda=6563Å) and the wavelength range of the last filter extends to z=0.047 (i.e., ∼200 Mpc). The first two filters (Ha1 and Ha2) make up the first filter pair and the 3rd and 4th filters (Ha3 and Ha4) make up the second filter pair. The survey uses an observational strategy of 3 spatially-staggered, overlapping grids that are limited to a declination of greater than -20°, where each grid contains N=3626 fields (26,470deg² of the sky). Observations using the Ha1 and Ha2 filters cover the entire sky above -20° declination. Observations using the Ha3 and Ha4 filters also cover the sky above -20° declination, but avoid the Galactic plane (\|b\| ≤ 3^deg). A single 60 second exposure is taken for each field in each grid resulting in three images for the majority of positions on the sky. Paper submitted: https://arxiv.org/pdf/1710.05016.pdf
Ref:	=2019ApJ...880....7C
by	COOK D.O. , KASLIWAL M.M., VAN SISTINE A., KAPLAN D.L., SUTTER J.S., KUPFER T., SHUPE D.L., LAHER R.R., MASCI F.J., DALE D.A., SESAR B., BRADY P.R., YAN L., OFEK E.O., REITZE D.H., KULKARNI S.R.
	Astrophys. J., 880, 7-7 (2019)
	Census of the Local Universe (CLU) narrowband survey. I. Galaxy catalogs from preliminary fields.
o	Table 2: <CLU JHHMMSS.ss+DDMMSS.s> N=793. Caltech/IPAC
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CLUST
CLUST	(Cluster)
*****	Avoid the usage of CLUST, prefer [ME95]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CLV96]
[CLV96]	(Conti+Leitherer+Vacca, 1996)
Write:	<<[CLV96] NGC 1741 A>> <<[CLV96] NGC 1741 AN>>
N:	3
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST FOC and GHRS observations
in source:	NGC 1741
Ref:	=1996ApJ...461L..87C
by	CONTI P.S. , LEITHERER C., VACCA W.D.
	Astrophys. J., 461, 87-90 (1996)
	Hubble Space Telescope ultraviolet spectroscopy of NGC 1741: a nearby template for distant energetic starbursts.
o	<[CLV96] NGC 1741 A> (Nos A-B), <[CLV96] NGC 1741 AN> No. B1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLW2011]
[CLW2011]	(Chies-Santos+Larsen+Wehner+, 2011)
Write:	<<[CLW2011] NGC NNNN NNN>>
N:	1301
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	WHT LIRIS observations of N=1301 globular clusters in 14 bright nearby early-type galaxies. Use of HST ACS archival images.
Ref:	=2011A&A...525A..19C
by	CHIES-SANTOS A.L. , LARSEN S.S., WEHNER E.M., KUNTSCHNER H., STRADER J., BRODIE J.P.
	Astron. Astrophys., 525A, 19-19 (2011)
	An optical/NIR survey of globular clusters in early-type galaxies. I. Introduction and data reduction procedures.
o	Table 4: <[CLW2011] NGC NNNN NNN> N=1301.
=E=	Catalogue in electronic form as J/A+A/525/A19
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLW2016]
[CLW2016]	(Csengeri+Leurini+Wyrowski+, 2016)
Write:	<<[CLW2016] GLL.ll+B.bbA>>
N:	430
Object:	Clump (SIMBAD class: MolCld = Molecular Cloud)
Note:	IRAM 30m telescope and APEX SiO(2-1) and SiO(5-4) line observations of N=430 massive clumps in the inner Galaxy. Use of the APEX Telescope Large Area Survey of the Galaxy (ATLASGAL).
Ref:	=2016A&A...586A.149C
by	CSENGERI T. , LEURINI S., WYROWSKI F., URQUHART J.S., MENTEN K.M., WALMSLEY M., BONTEMPS S., WIENEN M., BEUTHER H., MOTTE F., NGUYEN-LUONG Q., SCHILKE P., SCHULLER F., ZAVAGNO A., SANNA C.
	Astron. Astrophys., 586A, 149-149 (2016)
	ATLASGAL-selected massive clumps in the inner Galaxy. II. Characterisation of different evolutionary stages and their SiO emission.
o	Tables 4,6-7: <[CLW2016] GLL.ll+b.bbA> N=430.
=E=	Catalogue in electronic form as J/A+A/586/A149
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLW2020]
[CLW2020]	(Cheng+Li+Wang+, 2020)
Write:	<<[CLW2020] NNN>>
N:	300
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	N=300 X-ray sources in ω Cen. Use of archival Chandra data. See also [CLF2019], [CLL2019], [CML2020].
in source:	NGC 5139 = ome Cen
Ref:	=2020ApJ...904..198C
by	CHENG Z. , LI Z., WANG W., LI X., XU X.
	Astrophys. J., 904, 198-198 (2020)
	Exploring the mass segregation effect of X-ray sources in globular clusters. IV. Evidence of black hole burning in ω Centauri.
o	Table 1: <[CLW2020] NNN> (Nos 1-300).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [CLW98]
[CLW98]	(Chen+Lanzetta+Webb+, 1998)
Write:	<<[CLW98] HHMM+DDMM +xxxxx+yyyyy>>
N:	87+145
Object:	G (SIMBAD class: Galaxy)
Note:	WFPC2 WFPC2 images of galaxies in 28 fields 'HHMM+DDMM'. Maps.
Ref:	=1998ApJ...498...77C
by	CHEN H.-W. , LANZETTA K.M., WEBB J.K., BARCONS X.
	Astrophys. J., 498, 77-94 (1998)
	The gaseous extent of galaxies and the origin of Lyα absorption systems. III. Hubble space telescope imaging of Lyα-absorbing galaxies at z < 1.
o	Fig.1, Table 4: <[CLW98] HHMM+DDMM +xxxxx+yyyyy> N=87
Ref:	=2001ApJ...559..654C
by	CHEN H.-W. , LANZETTA K.M., WEBB J.K., BARCONS X.
	Astrophys. J., 559, 654-674 (2001)
	The gaseous extent of galaxies and the origin of Lyα absorption systems. V. Optical and near-infrared photometry of lyα-absorbing galaxies at z<1.
o	Table 3: <[CLW98] HHMM+DDMM +xxxxx+yyyyy> N=145 added.
=E=	Catalogue in electronic form as J/ApJ/559/654
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLX2015]
[CLX2015]	(Chen+Liu+Xiang+, 2015)
Write:	<<[CLX2015] LAMOST-N>> <<[CLX2015] LAMOST-CNN>>
N:	5+23
Object:	GlCl + Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Stat:	is completely incorporated in Simbad
Note:	Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) observations of N=5 globular clusters candidates in the halo of M31 and M33. Use of archival SDSS images.
in source:	M 31 = NGC 224
in source:	M 33 = NGC 598
Ref:	=2015RAA....15.1392C
by	CHEN B.-Q. , LIU X.-W., XIANG M.-S., YUAN H.-B., HUANG Y., HUO Z.-Y., SUN N.-C., WANG C., REN J.-J., ZHANG H.-W., REBASSA-MANSERGAS A., YANG M., ZHANG Y., HOU Y.-H., WANG Y.-F.
	RAA, 15, 1392-1413 (2015)
	The LAMOST spectroscopic survey of globular clusters in M 31 and M 33. I. catalog and new identifications.
o	Table 2: <[CLX2015] LAMOST-N> (Nos 1-5). Table 3: <[CLX2015] LAMOST-CNN> (Nos 01-23).
=E=	Catalogue in electronic form as J/other/RAA/15.1392
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLY2008]
[CLY2008]	(Chynoweth+Langston+Yun+, 2008)
Write:	<<[CLY2008] N>> <<[CLY2008] C08-N>> (not recognised by Simbad, but found in literature)
N:	5
Object:	HI Cloud (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	GBT HI observations of the M81-M82 group. See also [CLH2009], [CLH2011].
in source:	NAME M 81 GROUP
Ref:	=2008AJ....135.1983C
by	CHYNOWETH K.M. , LANGSTON G.I., YUN M.S., LOCKMAN F.J., RUBIN K.H.R., SCOLES S.A.
	Astron. J., 135, 1983-1992 (2008)
	Neutral hydrogen clouds in the M81/M82 group.
o	Table 5: <[CLY2008] N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CLZ2017]
[CLZ2017]	(Ching+Lai+Zhang+, 2017)
Write:	<<[CLZ2017] Cyg-NNN>>
N:	6
Object:	Dense Core (SIMBAD class: denseCore = Dense Core)
Note:	SMA 870µm observations of N=6 massive dense cores in the DR21 filament. See also [MBS2007c].
in source:	NAME Cyg X
Ref:	=2017ApJ...838..121C
by	CHING T.-C. , LAI S.-P., ZHANG Q., GIRART J.M., QIU K., LIU H.B.
	Astrophys. J., 838, 121-121 (2017)
	Magnetic fields in the massive dense cores of the DR21 filament: weakly magnetized cores in a strongly magnetized filament.
o	Table 2: <[CLZ2017] Cyg-NNN> N=6 among (Nos N38-N53).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CM
CM	(Crillon+Monnet)
*****	Avoid the usage of CM, prefer [CM69]
Origin	of the Acronym: L (1997AJ....113.1678B,1999A&A...345..778G)
Details on Acronym: CM
CM	(Conti+Massey)
*****	Avoid the usage of CM, prefer [CM81]
Origin	of the Acronym: L (1998ApJ...505..793M)
Details on Acronym: CM
CM	(Cappi+Maurogordato)
*****	Avoid the usage of CM, prefer [CM92]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CM2000]
[CM2000]	(Codella+Moscadelli, 2000) (Not yet in Simbad)
Write:	<<[CM2000] CH3OH LL.lll+B.bbb>> <<[CM2000] H2O LL.lll+B.bbb>>
N:	17+2
Object:	Maser (SIMBAD class: Maser)
Ref:	=2000A&A...362..723C
by	CODELLA C. , MOSCADELLI L.
	Astron. Astrophys., 362, 723-729 (2000)
	On the occurrence of the 6.7GHz CH_{3}OH maser emission in UCHII regions.
o	Table 1: <[CM2000] CH3OH LL.lll+B.bbb> N=17. Table 2: <[CM2000] H2O LL.lll+B.bbb> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CM2004]
[CM2004]	(Chamaraux+Masnou, 2004)= ([CM2004a])
Write:	<<[CM2004] NN>>
N:	12
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=12 groups of galaxies with the list of members in each group.
Ref:	=2004MNRAS.347..541C
by	CHAMARAUX P. , MASNOU J.-L.
	Mon. Not. R. Astron. Soc., 347, 541-555 (2004)
	Spatial distribution of galaxies in the Puppis region.
o	Table 3: <[CM2004] NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CM2004a]
[CM2004a]	(Chamaraux+Masnou, 2004)
*****	Avoid the usage of [CM2004a], prefer [CM2004]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CM2004b]
[CM2004b]	(Chen+Marzke, 2004)
Write:	<<[CM2004b] NNNNN>>
N:	9
Object:	G (SIMBAD class: Galaxy)
Note:	Identification of 9 early-type red galaxies in the HUDF NICMOS region.
in source:	NAME HUDF
Ref:	=2004ApJ...615..603C
by	CHEN H.-W. , MARZKE R.O.
	Astrophys. J., 615, 603-609 (2004)
	Discovery of massive evolved galaxies at z > 3 in the Hubble Ultra Deep Field.
o	Table 1: <[CM2004b] NNNNN> N=9 among N>12183.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CM2005]
[CM2005]	(Cohen+Melendez, 2005)
Write:	<<[CM2005] M13 CMMSSs-MMSS>> <<[CM2005] M3 CMMSSs-MMSS>>
N:	14+3
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Sample of stars in M 3 and M 13: spectra obtained with HIRES at the Keck observatory. In the format, coordinates are J2000, with for M 13: RA +16h, Dec +36deg, for M 3: RA +13h, Dec +28deg.
in source:	M 13 = NGC 6205
in source:	M 3 = NGC 5272
Ref:	=2005AJ....129..303C
by	COHEN J.G. , MELENDEZ J.
	Astron. J., 129, 303-329 (2005)
	Abundances in a large sample of stars in M3 and M13.
o	In the format, coordinates are J2000, with for M 13: RA +16h, Dec +36°, for M 3: RA +13h, Dec +28°.
o	Tables 1A, 4: <[CM2005] M13 CMMSSs-MMSS> N=14. Table 1B: <[CM2005] M3 CMMSSs-MMSS> N=3.
=E=	Catalogue in electronic form as J/AJ/129/303
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CM2006]
[CM2006]	(Chiboucas+Mateo, 2006)
Write:	<<[CM2006] JHHMMSS.ss+DDMMSS.ss>>
N:	78
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	LCO 1m telescope photometry and 2.5m telescope spectroscopy. Photometric observations of the core of ACO 3526 = Centaurus cluster.
in source:	ACO 3526 = Centaurus Cluster
Ref:	=2006AJ....132..347C
by	CHIBOUCAS K. , MATEO M.
	Astron. J., 132, 347-359 (2006)
	The luminosity function of nearby galaxy clusters. II. Redshifts and luminosity function for galaxies in the region of the Centaurus cluster.
o	Table 2: <[CM2006] JHHMMSS.ss+DDMMSS.ss> N=78.
=E=	Catalogue in electronic form as J/AJ/132/347
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CM2007]
[CM2007]	(Chiboucas+Mateo, 2007)
Write:	<<[CM2007] NNNN>>
N:	4667
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	LCO 1m telescope photometry. Catalog of galaxies within the central region of ACO 3526 = Centaurus Cluster.
in source:	Centaurus Cluster = ACO 3526
Ref:	=2007ApJS..170...95C
by	CHIBOUCAS K. , MATEO M.
	Astrophys. J., Suppl. Ser., 170, 95-107 (2007)
	The luminosity function of nearby galaxy clusters. I. A catalog of galaxies within the central 0.83 square ° of the Centaurus cluster.
o	Table 4: <[CM2007] NNNN> (Nos 1-4667).
=E=	Catalogue in electronic form as J/ApJS/170/95
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CM2009]
[CM2009]	(Chapman+Mundy, 2009)= ([CM2009a])
Write:	<<[CM2009] NN>>
N:	10
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	Spitzer (IRAC and MIPS) and KPNO Flamingos observations of the dense cores L1152 and L1228.
in source:	LDN 1152
in source:	LDN 1228
Ref:	=2009ApJ...699.1866C
by	CHAPMAN N.L. , MUNDY L.G.
	Astrophys. J., 699, 1866-1882 (2009)
	Deep JHK_{s} and Spitzer imaging of four isolated molecular cloud cores.
o	Tables 4-5: <[CM2009] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CM2009a]
[CM2009a]	(Chapman+Mundy, 2009)
*****	Avoid the usage of [CM2009a], prefer [CM2009]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CM2009b]
[CM2009b]	(Chen+Mulchaey, 2009) (Not yet in Simbad)
Write:	<<[CM2009b] PG1216+069 abs N.NNNNN>> <<[CM2009b] HE0226-4110 NNNNN>> <<[CM2009b] PG1216+069 NNNNN>>
N:	66+1793+1619
Object:	Absorber + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Magellan Baade Telescope IMACS observations of the fields around HE0226-4110 and PG1216+069.
Ref:	=2009ApJ...701.1219C
by	CHEN H.-W. , MULCHAEY J.S.
	Astrophys. J., 701, 1219-1242 (2009)
	Probing the intergalactic medium-galaxy connection at z < 0.5. I. A galaxy survey in QSO fields and a galaxy-absorber cross-correlation study.
o	Table 3: <[CM2009b] PG1216+069 abs N.NNNNN> N=66. Table 4: <[CM2009b] HE0226-4110 NNNNN> N=1793 among (Nos 443-16017). Table 6: <[CM2009b] PG1216+069 NNNNN> N=1619 among (Nos 539-24238).
=E=	Catalogue in electronic form as <J/ApJ/701/1219/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CM69]
[CM69]	(Crillon+Monnet, 1969)= (CM)
Write:	<<[CM69] NGC 4449 NN>> <<[CM69] NGC 4631 NN>>
N:	51+88
Object:	HII (SIMBAD class: HIIReg = HII Region)
in source:	NGC 4449
in source:	NGC 4631
Ref:	=1969A&A.....1..449C
by	CRILLON R. , MONNET G.
	Astron. Astrophys., 1, 449-451 (1969)
	Etude cinematique de l'hydrogene ionise dans NGC 4449.
o	Table 3: <[CM69] NGC 4449 NN> (Nos 1-51).
Ref:	=1969A&A.....2....1C
by	CRILLON R. , MONNET G.
	Astron. Astrophys., 2, 1-5 (1969)
	Etude cinematique de l'hydrogene ionise dans NGC 4631.
o	Table 3: <[CM69] NGC 4631 NN> (Nos 1-88).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CM81]
[CM81]	(Conti+Massey, 1981)= (CM)
Write:	<<[CM81] NN>>
N:	14
Object:	WR (SIMBAD class: WolfRayet* = Wolf-Rayet)
Stat:	is completely incorporated in Simbad
in source:	M 33 = NGC 598
Ref:	=1981ApJ...249..471C
by	CONTI P.S. , MASSEY P.
	Astrophys. J., 249, 471-480 (1981)
	Wolf-Rayet stars and giant HII regions in M 33: casual associations or meaningful relationships ?
o	<[CM81] NN> (Nos 1-14).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [CM82]
[CM82]	(Condon+Mitchell, 1982)
Write:	<<[CM82] NNA>>
N:	71
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA 1.4GHz continuum observations of extragalactic sources. Paper II, see also papers I: [CCH82] and III: [CCH85].
Ref:	=1982AJ.....87.1429C
by	CONDON J.J. , MITCHELL K.J.
	Astron. J., 87, 1429-None (1982)
	Complete samples of active extragalactic objects. II. A deep 1.452-GHz VLA survey centered on 08:52:15+17:16.
o	Table I: <[CM82] NNA> (Nos 1-66) N=71.
=E=	Catalogue in electronic form as J/AJ/87/1429
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CM84]
[CM84]	(Condon+Mitchell, 1984)
Write:	<<[CM84] NNNA>>
N:	168
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-159), format 'NNNA' 1993MNRAS.263..123R and 1993MNRAS.263...98B
Ref:	=1984AJ.....89..610C
by	CONDON J.J. , MITCHELL K.J.
	Astron. J., 89, 610-617 (1984)
	A deeper VLA survey of the alf = 08h52m15s, del = +17 16 field.
o	Table I: <[CM84] NNNA> (Nos 1-159) N=166
Ref:	=1985AJ.....90.1431C
by	COLEMAN P.H. , CONDON J.J.
	Astron. J., 90, 1431-1436 (1985)
	A high-resolution VLA survey of the alf = 08h52m15s, del +17 16 field.
o	Table I: <[CM84] NNNA> (Nos 37A-37B, 38A-38B, 85A-85B) added
Ref:	=1993MNRAS.263..123R
by	ROWAN-ROBINSON M. , BENN C.R., LAWRENCE A., McMAHON R.G., BROADHURST T.J.
	Mon. Not. R. Astron. Soc., 263, 123-130 (1993)
	The evolution of faint radio sources.
o	<[CM84] 143A> added
Ref:	=1993MNRAS.263...98B
by	BENN C.R. , ROWAN-ROBINSON M., McMAHON R.G., BROADHURST T.J., LAWRENCE A.
	Mon. Not. R. Astron. Soc., 263, 98-122 (1993)
	Spectroscopy of faint radio sources: the nature of the sub-mJy radio-source population.
o	<[CM84] 143B> added
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CM92]
[CM92]	(Cappi+Maurogordato, 1992)= (CM)
Write:	<<[CM92] WNNa>>
N:	24
Object:	Supercluster of G (SIMBAD class: SuperClG = Supercluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table 2: (N1-N11) Northern clusters, Table 3: (S1-S13) Southern clusters
Ref:	=1992A&A...259..423C
by	CAPPI A. , MAUROGORDATO S.
	Astron. Astrophys., 259, 423-434 (1992)
	The spatial distribution of nearby galaxy clusters in the northern and southern galactic hemispheres.
o	Table 2: <[CM92] ANN> (Nos N1-N11), Table 3: <[CM92] ANN> (Nos S1-S13)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CM95]
[CM95]	(Caselli+Myers, 1995)
Write:	<<[CM95] Ori BN>> <<[CM95] Ori ANN>>
N:	9+15
Object:	Core (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Tables 2: Massive cores in Ori B, format 'Ori BN', N=9, and in Ori A, format 'Ori ANN', N=15
in source:	NAME Ori A
in source:	NAME Ori B
Ref:	=1995ApJ...446..665C
by	CASELLI P. , MYERS P.C.
	Astrophys. J., 446, 665-686 (1995)
	The line width-size relation in massive cloud cores.
o	Table 2: <[CM95] Ori BN> (Nos B1-B9), <[CM95] Ori ANN> (Nos A1-A15)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CMa
CMa	(Canis Majoris)
*****	Avoid the usage of CMa, prefer [MWC53]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CMa R1
CMa R1	(CMa R1 Assoc.)
*****	Avoid the usage of CMa R1, prefer HRW
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CMA2011]
[CMA2011]	(Chernyakova+Malyshev+Aharonian+, 2011)
Write:	<<[CMA2011] DDD.ddd+DD.ddd>>
N:	4
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Fermi-LAT observations of the field of 1FGL J1745.6-2900.
Ref:	=2011ApJ...726...60C
by	CHERNYAKOVA M. , MALYSHEV D., AHARONIAN F.A., CROCKER R.M., JONES D.I.
	Astrophys. J., 726, 60 (2011)
	The high-energy, arcminute-scale galactic center γ-ray source.
o	Table 1: <[CMA2011] DDD.ddd+DD.ddd> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMB2006]
[CMB2006]	(Comerford+Meneghetti+Bartelmann+, 2006)
Write:	<<[CMB2006] ACO 370 GN>> <<[CMB2006] ClG 0054-27 GN>> <<[CMB2006] ClG 0939+4713 GN>>
N:	2+2+3
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Lens galaxies in N=3 clusters. Use of archival HST images.
in source:	ACO 370
in source:	ClG 0054-27
in source:	ClG 0939+4713 = ACO 851
Ref:	=2006ApJ...642...39C
by	COMERFORD J.M. , MENEGHETTI M., BARTELMANN M., SCHIRMER M.
	Astrophys. J., 642, 39-47 (2006)
	Mass distributions of Hubble Space Telescope galaxy clusters from gravitational arcs.
o	Table 1: <[CMB2006] ACO 370 GN> (Nos G1-G2), <[CMB2006] ClG 0054-27 GN> (Nos G1-G2), <[CMB2006] ClG 0939+4713 GN> (Nos G1-G3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMB2010]
[CMB2010]	(Choudhury+Mookerjea+Bhatt+, 2010)
Write:	<<[CMB2010] MIR-NNN>> <<[CMB2010] NIR-NN>>
N:	110+13
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Himalayan Chandra 2m telescope (HCT, India) HFOSC observations of SFO 38. Use of Spitzer IRAC And MIPS observations.
in source:	SFO 38
Ref:	=2010ApJ...717.1067C
by	CHOUDHURY R. , MOOKERJEA B., BHATT H.C.
	Astrophys. J., 717, 1067-1083 (2010)
	Triggered star formation and young stellar population in bright-rimmed cloud SFO 38.
o	Table 1: <[CMB2010] MIR-NNN> (Nos 1-110). Table 2: <[CMB2010] NIR-NN> (Nos 1-13).
=E=	Catalogue in electronic form as <J/ApJ/717/1067/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMB96]
[CMB96]	(Castellani+Marconi+Buonanno, 1996) (Not yet in Simbad)
Write:	<<[CMB96] NNN>>
N:	940
Object:	* (SIMBAD class: Star)
in source:	NAME Tucana Dwarf Galaxy
Ref:	=1996A&A...310..715C
by	CASTELLANI M. , MARCONI G., BUONANNO R.
	Astron. Astrophys., 310, 715-721 (1996)
	The Tucana dwarf Galaxy.
o	Table 2: <[CMB96] NNN> (Nos 1-940).
=E=	Catalogue in electronic form as J/A+A/310/715
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMB97]
[CMB97]	(Calzetti+Meurer+Bohlin+, 1997)= (C)
Write:	<<[CMB97] NGC 5253-NNa>>
N:	11+1
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations.
in source:	NGC 5253
Ref:	=1997AJ....114.1834C
by	CALZETTI D. , MEURER G.R., BOHLIN R.C., GARNETT D.R., KINNEY A.L., LEITHERER C., STORCHI-BERGMANN T.
	Astron. J., 114, 1834-1849 (1997)
	Dust and recent star formation in the core of NGC 5253.
o	Table 3: cross-id. UV = [MHL95] NGC 5253 NN
o	Table 3: <[CMB97] NGC 5253-N> (Nos 1-6)
Ref:	=2001ApJ...555..322T
by	TREMONTI C.A. , CALZETTI D., LEITHERER C., HECKMAN T.M.
	Astrophys. J., 555, 322-337 (2001)
	Star formation in the field and clusters of NGC 5253.
o	Table 1: <[CMB97] NGC 5253-NN> (Nos 7-11) added.
Ref:	=2004A&A...415..509V
by	VANZI L. , SAUVAGE M.
	Astron. Astrophys., 415, 509-520 (2004)
	Dust and super star clusters in NGC 5253.
o	Fig.1, Table 1: <[CMB97] NGC 5253-NNa> (No. 5a) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CMC
CMC	(Carlsberg Meridian Catalogues)= CAMC
Write:	<<CMC NNNNNN>>
N:	about 800000
Object:	* (SIMBAD class: Star)
Note:	8 catalogues (CMC1 to CMC8), available on magnetic tape. 4th volume supersedes the first three volumes.
Ref:	=1993BICDS..42....5F
by	FABRICIUS C.
	Bull. Inf. Centre Donnees Stellaires, 42, 5-9 (1993)
	The Carlsberg meridian catalogues.
o	<CMC NNNNNN> N about 800000
=E=	Catalogue in electronic form as I/147
=E=	Catalogue in electronic form as I/170
=E=	Catalogue in electronic form as I/189
=E=	Catalogue in electronic form as I/205
=E=	Catalogue in electronic form as I/213
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CMC14
CMC14	(Carlsberg Meridian Catalog 14)
Write:	<<CMC14 JHHMMSS.s+DDMMSS>>
N:	95858475
Object:	* (SIMBAD class: Star)
Note:	Carlsberg Meridian Telescope observations.
Ref:	=2006yCat.1304....0C
by	COPENHAGEN UNIVERSITY OBSERVATORY , (The Cambridge Institute of Astronomy), (The Real Instituto y Observatorio de la Armada en San Fernando)
	yCat, 1304, 0 (2006)
	Carlsberg Meridian Catalog 14 (CMC14) (CMC, 2006).
o	<CMC14 JHHMMSS.s+DDMMSS> N=95858475.
=E=	Catalogue in electronic form as I/304
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CMC2000]
[CMC2000]	(Churchill+Mellon+Charlton+, 2000)= ([CMC2000a])
Write:	<<[CMC2000] QSO JHHMM+DDMM abs N.NNNN>>
N:	45
Object:	Absorber
Note:	HIRES-Keck absorption line systems for 17 QSOs.
Ref:	=2000ApJS..130...91C
by	CHURCHILL C.W. , MELLON R.R., CHARLTON J.C., JANNUZI B.T., KIRHAKOS S., STEIDEL C.C., SCHNEIDER D.P.
	Astrophys. J., Suppl. Ser., 130, 91-119 (2000)
	Low- and high-ionization absorption properties of Mg II absorption-selected galaxies at intermediate redshifts. I. General properties.
o	Table 3: <[CMC2000] QSO JHHMM+DDMM abs N.NNNN> N=45.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMC2000a]
[CMC2000a]	(Churchill+Mellon+Charlton+, 2000)
*****	Avoid the usage of [CMC2000a], prefer [CMC2000]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMC2000b]
[CMC2000b]	(Clark+McCall+Chrysostomou+, 2000) (Not yet in Simbad)
Write:	<<[CMC2000b] A>>
N:	6
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Fig.4: (Nos A-F), Features in R CrA and T CrA system. See also [WWS85].
Ref:	=2000MNRAS.319..337C
by	CLARK S. , McCALL A., CHRYSOSTOMOU A., GLEDHILL T., YATES J., HOUGH J.
	Mon. Not. R. Astron. Soc., 319, 337-349 (2000)
	Polarization models of young stellar objects - II. Linear and circular polarimetry of R Coronae Australis.
o	Fig.4: <[CMC2000b] A> (Nos A-F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMC2005]
[CMC2005]	(Carraro+Mendez+Costa, 2005)
Write:	<<[CMC2005] NGC NNNN NNNNN>>
N:	24295+26086
Object:	* (SIMBAD class: Star)
Note:	Las Campanas Observatory Warsaw 1.3m telescope observations of the open clusters NGC 6404 and NGC 6583.
in source:	NGC 6404
in source:	NGC 6583
Ref:	=2005MNRAS.356..647C
by	CARRARO G. , MENDEZ R.A., COSTA E.
	Mon. Not. R. Astron. Soc., 356, 647-653 (2005)
	NGC 6404 and 6583: two neglected intermediate-age open clusters located in the Galactic Centre direction.
o	<[CMC2005] NGC 6404 NNNNN> (Nos 1-24295). <[CMC2005] NGC 6583 NNNNN> (Nos 1-26086).
o	Table 1: PG 2213+006 is a misprint for PG 2213-006. In chap. 5.2 : NGC 6503 is a misprint for NGC 6583.
=E=	Catalogue in electronic form as <J/MNRAS/356/647/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMC2011]
[CMC2011]	(Curran+Maccarone+Casella+, 2011)
Write:	<<[CMC2011] A>>
N:	2
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Swift UVOT observations of N=2 possible counterparts of XTE J1752-223.
Ref:	=2011MNRAS.410..541C
by	CURRAN P.A. , MACCARONE T.J., CASELLA P., EVANS P.A., LANDSMAN W., KRIMM H.A., BROCKSOPP C., STILL M.
	Mon. Not. R. Astron. Soc., 410, 541-547 (2011)
	Black hole candidate XTE J1752-223: Swift observations of canonical states during outburst.
o	Fig. 1: <[CMC2011] A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMC2016]
[CMC2016]	(Civano+Marchesi+Comastri+, 2016)
Write:	<<[CMC2016] lid NNNNN>> <<[CMC2016] lid_NNNNN>> (not recognised by Simbad, but found in literature)
N:	2273
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-I observations of N=2273 X-ray point sources, as part of the COSMOS-Legacy survey. See also [ECV2009].
in source:	NAME COSMOS Field
Ref:	=2016ApJ...819...62C
by	CIVANO F. , MARCHESI S., COMASTRI A., URRY M.C., ELVIS M., CAPPELLUTI N., PUCCETTI S., BRUSA M., ZAMORANI G., HASINGER G., ALDCROFT T., ALEXANDER D.M., ALLEVATO V., BRUNNER H., CAPAK P., FINOGUENOV A., FIORE F., FRUSCIONE A., GILLI R., GLOTFELTY K., GRIFFITHS R.E., HAO H., HARRISON F.A., JAHNKE K., KARTALTEPE J., KARIM A., LAMASSA S.M., LANZUISI G., MIYAJI T., RANALLI P., SALVATO M., SARGENT M., SCOVILLE N.J., SCHAWINSKI K., SCHINNERER E., SILVERMAN J., SMOLCIC V., STERN D., TOFT S., TRAKHTENBROT B., TREISTER E., VIGNALI C.
	Astrophys. J., 819, 62 (2016)
	The Chandra Cosmos Legacy survey: overview and point source catalog.
o	Table 5: <[CMC2016] lid NNNNN> N=2273 among (Nos 38-10010).
=E=	Catalogue in electronic form as <J/ApJ/819/62/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMC2018]
[CMC2018]	(Casasola+Magrini+Combes+, 2018)= (CMC) = ([CMC2018a])
Write:	<<[CMC2018] CMC NN>>
N:	11
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	LBT LUCI near-infrared observations of N=11 galaxies in the field of the protocluster associated with 7C 1756+6520.
in source:	[GSS2010] 7C 1756+6520 cluster
Ref:	=2018A&A...618A.128C
by	CASASOLA V. , MAGRINI L., COMBES F., SANI E., FRITZ J., RODIGHIERO G., POGGIANTI B., BIANCHI S., LIUZZO E.
	Astron. Astrophys., 618A, 128-128 (2018)
	Spectroscopic characterization of the protocluster of galaxies around 7C 1756+6520 at z ~ 1.4.
o	Tables 1, A.1: <[CMC2018] CMC NN> (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMC2018a]
[CMC2018a]	(Casasola+Magrini+Combes+, 2018)= (CMC)
*****	Avoid the usage of [CMC2018a], prefer [CMC2018]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMC2018b]
[CMC2018b]	(Campusano+Marinello G.+Clowes+, 2018)
Write:	<<[CMC2018b] NNN>>
N:	341
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=341 galaxy clusters in the Northern and Southern Galactic Patches (NGP and SGP) of the Two-degree Field Galaxy Redshift Survey (2dFGRS), using a two-step algorithm (VoML+G).
Ref:	=2018ApJ...869..145C
by	CAMPUSANO L.E. , MARINELLO G., CLOWES R.G., HAINES C.P., PEREIRA S., PIZARRO D., HITSCHFELD-KAHLER N., SOCHTING I.K.
	Astrophys. J., 869, 145-145 (2018)
	A 3D Voronoi+Gapper galaxy cluster finder in Redshift space to z ~ 0.2. II. An abundant cluster population dominated by late-type galaxies unveiled.
o	Table 2: <[CMC2018b] NNN> (Nos 1-341).
=E=	Catalogue in electronic form as <J/ApJ/869/145/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMC2021]
[CMC2021]	(Carlin+Mutlu-Pakdil+Crnojevic+, 2021)
Write:	<<[CMC2021] MADCASH-N NNNN>>
N:	4807+2561
Object:	* (SIMBAD class: Star)
Note:	HST ACS observations of N=4807+2561 stars in the dwarf spheroidal galaxies MADCASH-1 and MADCASH-2.
in source:	MADCASH J074238+652501-dw
in source:	MADCASH J121007+352635-dw
Ref:	=2021ApJ...909..211C
by	CARLIN J.L. , MUTLU-PAKDIL B., CRNOJEVIC D., GARLING C.T., KARUNAKARAN A., PETER A.H.G., TOLLERUD E., FORBES D.A., HARGIS J.R., LIM S., ROMANOWSKY A.J., SAND D.J., SPEKKENS K., STRADER J.
	Astrophys. J., 909, 211-211 (2021)
	Hubble Space Telescope observations of two faint dwarf satellites of nearby LMC analogs from MADCASH.
o	<MADCASH JHHMMSS+DDMMSS-dw> N=2 = <MADCASH-N> (Nos 1-2). Table 1: <[CMC2021] MADCASH-1 NNNN> (Nos 0-4806). Table 2: <[CMC2021] MADCASH-2 NNNN> (Nos 0-2560).
=E=	Catalogue in electronic form as <J/ApJ/909/211/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CMCHerschel
CMCHerschel	(California Molecular Cloud Herschel)
Write:	<<CMCHerschel NNN>>
N:	300
Object:	Core (SIMBAD class: FarIR = Far-IR source (λ >= 30 µm))
Stat:	is completely incorporated in Simbad
Note:	N=300 cores from the H2 column density map based on Herschel 160 to 500µm in the California Molecular Cloud. Use of Herschel archival data.
Rem:	(a dash between the acronym and its contents is found in the literature)
in source:	NAME California Molecular Cloud
Ref:	=2018A&A...620A.163Z
by	ZHANG G.-Y. , XU J.-L., VASYUNIN A.I., SEMENOV D.A., WANG J.-J., DIB S., LIU T., LIU S.-Y., ZHANG C.-P., LIU X.-L., WANG K., LI D., WU Z.-Z., YUAN J.-H., LI D.-L., GAO Y.
	Astron. Astrophys., 620A, 163-163 (2018)
	Physical properties and chemical composition of the cores in the California molecular cloud.
o	cores.dat: <CMCHerschel NNN> (Nos 1-300).
=E=	Catalogue in electronic form as <J/A+A/620/A163/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CMD2007]
[CMD2007]	(Cresci+Mannucci+Della Valle+, 2007)
Write:	<<[CMD2007] Arp 220 SN>>
N:	1
Object:	Poss. SN (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST NICMOS image of Arp 220: discovery of a candidate SN
in source:	IC 4553 = APG 220
Ref:	=2007A&A...462..927C
by	CRESCI G. , MANNUCCI F., DELLA VALLE M., MAIOLINO R.
	Astron. Astrophys., 462, 927-931 (2007)
	A NICMOS search for obscured supernovae in starburst galaxies.
o	Appendix A, Fig.2: <[CMD2007] Arp 220 SN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMD2013]
[CMD2013]	(Chavarria-K.+Moreno-Corral+De Lara+, 2013)
Write:	<<[CMD2013] Star AN>> <<[CMD2013] Star a>> <<[CMD2013] Star IRAS06547-0810>> <<[CMD2013] Star NJHHMMSS.s+DDMMSS>>
N:	15+1+5
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	SPMO (Sierra San Pedro Martir National Astronomical Observatory) 0.84cm and 2.1m spectroscopy of the field of IRAS 06548-0815.
Ref:	=2013NewA...18...42C
by	CHAVARRIA-K C. , MORENO-CORRAL M.A., DE LARA E., DE LA FUENTE E.
	NewA, 18, 42-49 (2013)
	PMS and ZAMS stars associated with the dark cloud LDN 1655.
o	Fig. 2, Table 1: <[CMD2013] Star AN> (Nos A-J, i-k, G1, H1), <[CMD2013] Star IRAS06547-0810> N=1, <[CMD2013] NJHHMMSS.s+DDMMSS> N=5.
o	Star IRAS06547-0810 = UCAC2 28872585 in Simbad (the IRAS source is a double), and IRS 1 = 2MASS J06571429-0819450.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMD81]
[CMD81]	(Chanan+Margon+Downes, 1981)
Write:	<<[CMD81] HHMM+DDd>>
N:	19
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Ref:	=1981ApJ...243L...5C
by	CHANAN G.A. , MARGON B., DOWNES R.A.
	Astrophys. J., 243, 5-8 (1981)
	Optical identification of serendipitous Einstein sources: 19 X-ray-selected active galactic nuclei.
o	Table 1: <[CMD81] HHMM+DDd> N=19
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMD97]
[CMD97]	(Carpenter+Meyer+Dougados+, 1997)= (CMDSH)
Write:	<<[CMD97] NNNN>>
N:	512+390
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Stars in Mon R2 Cl*. Table 1: SQIID photometry (Nos 1001-1512) Table 2: IRCAM3 phtometry (Nos 1-390) See also [GMC98]
in source:	NAME Mon R2 Cluster
Ref:	=1997AJ....114..198C
by	CARPENTER J.M. , MEYER M.R., DOUGADOS C., STROM S.E., HILLENBRAND L.A.
	Astron. J., 114, 198-221 (1997)
	Properties of the Monoceros R2 stellar cluster.
o	(Erratum) Erratum AJ 114, p. 1225
o	Table 1: <[CMD97] NNNN> (Nos 1001-1512). Table 2: <[CMD97] NNN> (Nos 1-390)
=E=	Catalogue in electronic form as J/AJ/114/198
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CMDSH
CMDSH	(Carpenter+Meyer+Dougados+Strom+Hillebrand)
*****	Avoid the usage of CMDSH, prefer [CMD97]
Origin	of the Acronym: L (2003PASJ...55..635N)
Details on Acronym: [CME2001]
[CME2001]	(Cappi+Mazzotta+Elvis+, 2001)
Write:	<<[CME2001] RX J003033.2+261819 NN>> <<[CME2001] 3C 295 NN>> <<[CME2001] Anti-Leonid NN>> <<[CME2001] 3C 273 NN>>
N:	23+17+40+13
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra X-ray observatory observations of 4 fields: 2 ClG: RX J003033.2+261819 and NAME 3C 295 Cluster 2 comparison fields: Anti-Leonid and 3C 273.
in source:	RX J003033.0+261819
in source:	NAME 3C 295 Cluster
Ref:	=2001ApJ...548..624C
by	CAPPI M. , MAZZOTTA P., ELVIS M., BURKE D.J., COMASTRI A., FIORE F., FORMAN W., FRUSCIONE A., GREEN P., HARRIS D., HOOPER E.J., JONES C., KAASTRA J.S., KELLOGG E., MURRAY S., McNAMARA B., NICASTRO F., PONMAN T.J., SCHLEGEL E.M., SIEMIGINOWSKA A., TANANBAUM H., VIKHLININ A., VIRANI S., WILKES B.
	Astrophys. J., 548, 624-638 (2001)
	Chandra study of an overdensity of X-ray sources around two distant (z~0.5) clusters.
o	Table 2: <[CME2001] RX J003033.2+261819 NN> (Nos 1-23). Table 3: <[CME2001] 3C 295 NN> (Nos 1-17). Table 4: <[CME2001] Anti-Leonid NN> (Nos 1-40). Table 5: <[CME2001] 3C 273 NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMF84]
[CMF84]	(Cruz-Gonzalez+McBreen+Fazio, 1997) (Not yet in Simbad)
Write:	<<[CMF84] R>>
N:	2
Object:	(FIR) (SIMBAD class: Infrared = Infra-Red Source)
in source:	NAME R CrA Cloud
Ref:	=1984ApJ...279..679C
by	CRUZ-GONZALEZ I. , McBREEN B., FAZIO G.G.
	Astrophys. J., 279, 679-684 (1984)
	Far-infrared observations of a star-forming region in the Corona Australis dark cloud.
o	Table 1: <[CMF84] R> (Nos I-II)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CMFT
CMFT	(Cambresy+Marton+Feher+Toth)
Write:	<<CMFT NN>>
N:	2
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Use of UKIDSS DR8 of the Galactic Plane Survey to search for star clusters in the Rosette Molecular Cloud. See also [PL97], REFL.
in source:	NAME Rosette Molecular Complex
Ref:	=2013A&A...557A..29C
by	CAMBRESY L. , MARTON G., FEHER O., TOTH L.V., SCHNEIDER N.
	Astron. Astrophys., 557A, 29-29 (2013)
	Young stellar clusters in the Rosette Molecular Cloud. Arguments against triggered star formation.
o	Table 1: <CMFT NN> (Nos 10-11).
=E=	Catalogue in electronic form as <J/A+A/557/A29/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CMG2000]
[CMG2000]	(Callanan+McCarthy+Garcia, 2000) (Not yet in Simbad)
Write:	<<[CMG2000] N>>
N:	3
Object:	* (SIMBAD class: Star)
Note:	N=3 stars in the field of 4U 1630-47. Image in Figs 2, 3.
Ref:	=2000A&A...355.1049C
by	CALLANAN P.J. , McCARTHY J.F., GARCIA M.R.
	Astron. Astrophys., 355, 1049-1052 (2000)
	A search for the IR counterpart of the black hole candidate 4U 1630-47.
o	p. 1051, EXO 2040+375 misprint for 2030+375; GRO J1915+105 misprint for Granat 1915+105
o	Table 2: <[CMG2000] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMG2005]
[CMG2005]	(Corradi+Magrini+Greimel+, 2005)
Write:	<<[CMG2005] NGC NNN NN>>
N:	9+5+75
Object:	Poss. PN (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
Stat:	is completely incorporated in Simbad
Note:	Observations with the INT at La Palma. Search for PN candidates in 3 galaxies companions of M 31.
in source:	NGC 147
in source:	NGC 185
in source:	NGC 205 = M 110
Ref:	=2005A&A...431..555C
by	CORRADI R.L.M. , MAGRINI L., GREIMEL R., IRWIN M., LEISY P., LENNON D.J., MAMPASO A., PERINOTTO M., POLLACCO D.L., WALSH J.R., WALTON N.A., ZIJLSTRA A.A.
	Astron. Astrophys., 431, 555-563 (2005)
	The Local Group Census: planetary nebulae in the spheroidal galaxies NGC 147, NGC 185 and NGC 205.
o	Table 2: <[CMG2005] NGC 147 N> (Nos 1-9). Table 3: <[CMG2005] NGC 185 N> (Nos 1-5). Table 4: <[CMG2005] NGC 205 NN> (Nos 1-75).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMG2008]
[CMG2008]	(Campana+Massaro+Gasparrini+, 2008)
Write:	<<[CMG2008] DDD.dd+D.dd>>
N:	7
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	EGRET gamma-ray sources found with a minimal spanning tree (MST) algorithm.
Ref:	=2008MNRAS.383.1166C
by	CAMPANA R. , MASSARO E., GASPARRINI D., CUTINI S., TRAMACERE A.
	Mon. Not. R. Astron. Soc., 383, 1166-1174 (2008)
	A Minimal Spanning Tree algorithm for source detection in γ-ray images.
o	In Table 1 : BZQ J1236+0224 is probably a misprint for BZQ J1232-0224
o	Table 1: <[CMG2008] DDD.dd+D.dd> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMG2010]
[CMG2010]	(Chavarria+Mardones+Garay+, 2010)
Write:	<<[CMG2010] GLLL.lllA>>
N:	5
Object:	Assoc. (SIMBAD class: Association = Association of Stars)
Stat:	is completely incorporated in Simbad
Note:	VLT ISAAC observations of N=5 groups of NIR-excess sources toward four star-forming regions in the Norma spiral arm.
Ref:	=2010ApJ...710..583C
by	CHAVARRIA L. , MARDONES D., GARAY G., ESCALA A., BRONFMAN L., LIZANO S.
	Astrophys. J., 710, 583-596 (2010)
	Four highly luminous massive star-forming regions in the Norma spiral arm. II. Deep near-infrared imaging.
o	Fig. 7, Table 5: <[CMG2010] GLLL.lllA> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMG2014]
[CMG2014]	(Codella+Maury+Gueth+, 2014)
Write:	<<[CMG2014] MMN>>
N:	3
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	IRAM PdB observations of N=3 continuum sources associated with NGC 1333-IRAS2A.
in source:	NGC 1333:[JCC87] IRAS 2A = [JCC87] IRAS 2A
Ref:	=2014A&A...563L...3C
by	CODELLA C. , MAURY A.J., GUETH F., MARET S., BELLOCHE A., CABRIT S., ANDRE Ph.
	Astron. Astrophys., 563L, 3-3 (2014)
	First results from the CALYPSO IRAM-PdBI survey. III. Monopolar jets driven by a proto-binary system in NGC1333-IRAS 2A.
o	Fig. 1, Table 1: <[CMG2014] MMN> (Nos MM1-MM3).
=E=	Catalogue in electronic form as <J/A+A/563/L3/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMG2018]
[CMG2018]	(Contreras Ramos+Minniti+Gran+, 2018)
Write:	<<[CMG2018] bNNN NNN NNNNNN>> <<[CMG2018] bNNN_NNN_NNNNNN>> (not recognised by Simbad, but found in literature)
N:	960
Object:	Poss. RR Lyr (SIMBAD class: RRLyrae_Candidate = RR Lyrae Variable Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=960 RR Lyr candidates in deep near-IR images from the VISTA Variables in the Via Lactea (VVV) Survey within 100 arcmin from the Galactic Center (comprising VVV tiles b304, b305, b318, b319, b320, b332, b333, b334, b346, b347, and b348).
in source:	NAME Galactic Center
Ref:	=2018ApJ...863...79C
by	CONTRERAS RAMOS R. , MINNITI D., GRAN F., ZOCCALI M., ALONSO-GARCIA J., HUIJSE P., NAVARRO M.G., ROJAS-ARRIAGADA A., VALENTI E.
	Astrophys. J., 863, 79-79 (2018)
	The VVV Survey RR Lyrae population in the Galactic Center region.
o	Tables 1-2: <[CMG2018] bNNN NNN NNNNNN> N=960.
=E=	Catalogue in electronic form as <J/ApJ/863/79/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMG93]
[CMG93]	(Chu+Mac Low+Garcia-Seugura+, 1993)
Write:	<<[CMG93] Shell N>> <<[CMG93] SB>> <<[CMG93] ND>>
N:	3+2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations X-ray sources in LHA 120-N 44: N=3: areas of 'Shell 1', 'Shell 2' and 'Shell 3' with Shell 1 and 2 = [ML91] Shell 1 and 2 respectively. and N=2: SB = South Bar, and ND = North Diffuse See also [ML91]
in source:	Magellanic Clouds:LMC:LHA 120-N 44 = LHA 120-N 44
Ref:	=1993ApJ...414..213C
by	CHU Y.-H. , MAC LOW M.-M., GARCIA-SEGURA G., WAKKER B., KENNICUTT R.C.Jr
	Astrophys. J., 414, 213-218 (1993)
	Hidden supernova remnants in the Large Magellanic Cloud HII complex N 44.
o	Table 1: <[CMG93] Shell N> (Nos 1-3), <[CMG93] SB>, <[CMG93] ND>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMH2010]
[CMH2010]	(Cormier+Madden+Hony+, 2010) (Not yet in Simbad)
Write:	<<[CMH2010] NGC 4214-R>>
N:	3
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	Herschel PACS spectroscopic maps of the dwarf galaxy NGC 4214. Use of CO(1-0) contours from Walter et al. 2001AJ....121..727W. Regions NGC 4214-I and -II are centered on the [C II] peaks, while region NGC 4214-III was chosen by taking into account the peak of the CO emission.
in source:	NGC 4214
Ref:	=2010A&A...518L..57C
by	CORMIER D. , MADDEN S.C., HONY S., CONTURSI A., POGLITSCH A., GALLIANO F., STURM E., DOUBLIER V., FEUCHTGRUBER H., GALAMETZ M., GEIS N., DE JONG J., OKUMURA K., PANUZZO P., SAUVAGE M.
	Astron. Astrophys., 518L, 57-57 (2010)
	The effects of star formation on the low-metallicity ISM: NGC 4214 mapped with Herschel/PACS spectroscopy.
o	Fig. 2, Table 1: <[CMH2010] NGC 4214-R> (Nos I-III).
Details on Acronym: [CMH2019]
[CMH2019]	(Cuevas-Otahola+Mateu+Hernandez-Perez+, 2019)
Write:	<<[CMH2019] NNNNNNNN>>
N:	1125
Object:	EB* (SIMBAD class: EclBin = Eclipsing Binary)
Stat:	is completely incorporated in Simbad
Note:	N=1125 eclipsing binaries in the QUEST variability survey at low Galactic latitude.
Ref:	=2019MNRAS.484.2514C
by	CUEVAS-OTAHOLA B. , MATEU C., HERNANDEZ-PEREZ F., DOWNES J.J., VIVAS A.K., BRICENO C.
	Mon. Not. R. Astron. Soc., 484, 2514-2529 (2019)
	Eclipsing binary search in the QUEST low-latitude catalogue and the ELLISA light-curve simulator.
o	Table 3: <[CMH2019] NNNNNNNN> N=1125 among (Nos 40047541-80815591).
=E=	Catalogue in electronic form as <J/MNRAS/484/2514/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMI2001]
[CMI2001]	(Carrasco+Mendes de Oliveira+Infante+, 2001)
Write:	<<[CMI2001] NNNN-FF>> <<[CMI2001] NNNN-d-FF>> <<[CMI2001] LNN>>
N:	60+5+4
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Note:	Low Surface Brightness Dwarf galaxies (LSBD) in the Dorado group. In the format, the letter 'd' stands for 'deep' (N=5 additional larger diameter galaxies), the format 'LNN' for N=4 'Large' LSBD.
in source:	NAME DORADO GROUP
Ref:	=2001AJ....121..148C
by	CARRASCO E.R. , MENDES DE OLIVEIRA C., INFANTE L., BOLTE M.
	Astron. J., 121, 148-168 (2001)
	The dwarf galaxy population of the Dorado group down to M_{V}~-11.
o	Table 3: <[CMI2001] NNNN-FF> N=60, <[CMI2001] NNNN-d-FF> N=5, <[CMI2001] LNN> (Nos L01-L04).
=E=	Catalogue in electronic form as J/AJ/121/148
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMI2006]
[CMI2006]	(Chaty+Mignani+Israel, 2006)= ([CMI2006a]) (Not yet in Simbad)
Write:	<<[CMI2006] N>>
N:	2
Object:	(Near IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	CFHT Near-IR observations of XTE J1908+094: 2 possible counterpart are observed.
Ref:	=2006MNRAS.365.1387C
by	CHATY S. , MIGNANI R.P., ISRAEL G.L.
	Mon. Not. R. Astron. Soc., 365, 1387-1391 (2006)
	A closer look at the X-ray transient XTE J1908+094: identification of two new near-infrared candidate counterparts.
o	FIg.1, text: <[CMI2006] N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMI2006a]
[CMI2006a]	(Chaty+Mignani+Israel, 2006) (Not yet in Simbad)
*****	Avoid the usage of [CMI2006a], prefer [CMI2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMI2006b]
[CMI2006b]	(Carrasco+Mendes de Olivera+Infante, 2006)
Write:	<<[CMI2006b] H42-fNN-NNNN>> <<[CMI2006b] H42-fNN-LNN>> <<[CMI2006b] N5846-fNN-NNNN>> <<[CMI2006b] N5846-fNN-LNN>> <<[CMI2006b] IC 4765-fNN-NNNN>> <<[CMI2006b] IC 4765-fNN-LNN>> <<[CMI2006b] N6868-fNN-NNNN>> <<[CMI2006b] N6868-fNN-LNN>>
N:	32+16+20+12
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Note:	Photometry of 4 group of galaxies at the 1.3m Warsaw telescope at Las Campanas to search for LSB dwarf galaxies. Format: Name of the group + field name (fNN) + galaxy number (NNNN or LNN for LSB galaxies).
in source:	HCG 42
in source:	NAME NGC 5846 GROUP
in source:	NAME IC 4765 GROUP
in source:	NAME NGC 6868 GROUP
Ref:	=2006AJ....132.1796C
by	CARRASCO E.R. , MENDES DE OLIVEIRA C., INFANTE L.
	Astron. J., 132, 1796-1817 (2006)
	The dwarf galaxy population in nearby groups: the data.
o	Tables 3-4: <[CMI2006b] H42-fNN-NNNN> N=26+184, <[CMI2006b] N5846-fNN-NNNN> N=11+126, <[CMI2006b] IC 4765-fNN-NNNN> N=13+42, <[CMI2006b] N6868-fNN-NNNN> N=10+57. Table 3: <[CMI2006b] H42-fNN-LNN> N=6, <[CMI2006b] N5846-fNN-LNN> N=5, <[CMI2006b] IC 4765-fLNN> N=6, <[CMI2006b] N6868-fNN-LNN> N=2.
=E=	Catalogue in electronic form as J/AJ/132/1796
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMI2010]
[CMI2010]	(Cucciati+Marinoni+Iovino+, 2010)
Write:	<<[CMI2010] NNN>>
N:	318
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Catalogue of N=318 optical galaxy groups in the VIMOS-VLT deep redshift Survey (VVDS).
Ref:	=2010A&A...520A..42C
by	CUCCIATI O. , MARINONI C., IOVINO A., BARDELLI S., ADAMI C., MAZURE A., SCODEGGIO M., MACCAGNI D., TEMPORIN S., ZUCCA E., DE LUCIA G., BLAIZOT J., GARILLI B., MENEUX B., ZAMORANI G., LE FEVRE O., CAPPI A., GUZZO L., BOTTINI D., LE BRUN V., TRESSE L., VETTOLANI G., ZANICHELLI A., ARNOUTS S., BOLZONELLA M., CHARLOT S., CILIEGI P., CONTINI T., FOUCAUD S., FRANZETTI P., GAVIGNAUD I., ILBERT O., LAMAREILLE F., McCRACKEN H.J., MARANO B., MERIGHI R., PALTANI S., PELLO R., POLLO A., POZZETTI L., VERGANI D., PEREZ-MONTERO E.
	Astron. Astrophys., 520A, 42-42 (2010)
	The VIMOS-VLT deep survey: the group catalogue.
o	Tables 4-5: <[CMI2010] NNN> (Nos 1-318).
=E=	Catalogue in electronic form as J/A+A/520/A42
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMJ2007]
[CMJ2007]	(Chieregato+Miranda+Jetzer, 2007) (Not yet in Simbad)
Write:	<<[CMJ2007] A>>
N:	4
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	NAOS-CONICA image of QSO 0045-3337 field.
Ref:	=2007A&A...474..777C
by	CHIEREGATO M. , MIRANDA M., JETZER P.
	Astron. Astrophys., 474, 777-782 (2007)
	Q0045-3337: models including strong lensing by a spiral galaxy.
o	Figs 1, 3: <[CMJ2007] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMK2002]
[CMK2002]	(Caretta+Maia+Kawasaki+, 2002)= ([CMK2002a])
Write:	<<[CMK2002] Gal N>>
N:	5
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=5 galaxies used for calibration. See also AqrCC.
Ref:	=2002AJ....123.1200C
by	CARETTA C.A. , MAIA M.A.G., KAWASAKI W., WILLMER C.N.A.
	Astron. J., 123, 1200-1215 (2002)
	The Aquarius superclusters. I. Identification of clusters and superclusters.
o	Table 2: <[CMK2002] Gal N> (Nos 1-5). Table 3: <AqrCC NNN> (Nos 1-102).
=E=	Catalogue in electronic form as J/AJ/123/1200
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMK2002a]
[CMK2002a]	(Caretta+Maia+Kawasaki+, 2002)
*****	Avoid the usage of [CMK2002a], prefer [CMK2002]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMK2002b]
[CMK2002b]	(Courbin+Meylan+Kneib+, 2002) (Not yet in Simbad)
Write:	<<[CMK2002b] Lens SP>> <<[CMK2002b] Low-z Lens>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Note:	N=2 lens galaxies in PKS 1830-211 lensed system. In the format 'SP' stands for 'SPIRAL'. See also [LFK2000].
Ref:	=2002ApJ...575...95C
by	COURBIN F. , MEYLAN G., KNEIB J.-P., LIDMAN C.
	Astrophys. J., 575, 95-102 (2002)
	Cosmic alignment toward the radio Einstein ring PKS 1830-211?
o	Fig.3, Table 1: <[CMK2002b] Lens SP> N=1, <[CMK2002b] Low-z Lens> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMK99]
[CMK99]	(Chamaraux+Masnou+Kazes+, 1999)
Write:	<<[CMK99] AHHMMm+DDMM>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=2 galaxies not included in other catalogues.
Ref:	=1999MNRAS.307..236C
by	CHAMARAUX P. , MASNOU J.-L., KAZES I., SAITO M., TAKATA T., YAMADA T.
	Mon. Not. R. Astron. Soc., 307, 236-252 (1999)
	H I observations of galaxies behind the Milky Way in the Puppis region.
o	Table 1: <[CMK99] AHHMMm+DDMM> N=2.
=E=	Catalogue in electronic form as J/MNRAS/307/236
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CML2020]
[CML2020]	(Cheng+Mu+Li+, 2020) (Not yet in Simbad)
Write:	<<[CML2020] NNN>>
N:	502
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	N=502 X-ray sources in the bulge of the globular cluster M28. Use of archival Chandra data. See also [CLF2019], [CLL2019], [CLW2020].
in source:	NGC 6626 = M 28
Ref:	=2020ApJ...892...16C
by	CHENG Z. , MU H., LI Z., XU X., WANG W., LI X.
	Astrophys. J., 892, 16-16 (2020)
	Exploring the mass segregation effect of X-ray sources in globular clusters. III. Signs of binary disruption in M28.
o	Table 2: <[CML2020] NNN> (Nos 1-502).
=E=	Catalogue in electronic form as <J/ApJ/892/16/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CML98]
[CML98]	(Castro-Tirado+Metcalfe+Laureijs+, 1998)= ([CML98a])
Write:	<<[CML98] NN>> <<[CML98] A>>
N:	47+4
Object:	* + G (SIMBAD class: Infrared = Infra-Red Source)
Note:	ISO CAM and PHT observations Table 2: IR sources detected in GRB 970402 field, (Nos 1-47), 40 , 2 poss. , 4 G, 1 poss. G Table 3: N=4 other sources (Nos A-D), in the error box of SAX J1450.1-6920, 2 *, 1 G, 1 ? Identif. chart in Fig.2
Ref:	=1998A&A...330...14C
by	CASTRO-TIRADO A.J. , METCALFE L., LAUREIJS R., ALTIERI B., GOROSABEL J., HANLON L., McBREEN B., SMITH N., COSTA E., FEROCI M., PALAZZI E., NICASTRO L., FRONTERA F., CLARET A., KESSLER M.
	Astron. Astrophys., 330, 14-18 (1998)
	ISO observations of the GRB 970402 error box.
o	Table 2: <[CML98] NN> (Nos 1-47). Table 3: <[CML98] A> (Nos A-D)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CML98a]
[CML98a]	(Castro-Tirado+Metcalfe+Laureijs+, 1998)
*****	Avoid the usage of [CML98a], prefer [CML98]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CML98b]
[CML98b]	(Clayton+Meaburn+Lopez+, 1998)
Write:	<<[CML98b] SN>>
N:	2
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	See also [MW86]
in source:	NAME Rosette Nebula
Ref:	=1998A&A...334..264C
by	CLAYTON C.A. , MEABURN J., LOPEZ J.A., CHRISTOPOULOU P.E., GOUDIS C.D.
	Astron. Astrophys., 334, 264-268 (1998)
	Imaging studies of localized, ionized flows in the Rosette nebula.
o	Knot B and Knot C = [MW86] Rosette Knot B and [MW86] Rosette Knot C
o	<[CML98b] SN> (Nos S1-S2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMM2004]
[CMM2004]	(Coia+McBreen+Metcalfe+, 2004)= (ISO) (Not yet in Simbad)
Write:	<<[CMM2004] NN>>
N:	44
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	ISO observations of the cluster ClG 0024+1652.
in source:	ClG 0024+1652 = HMS 0024+1654
Ref:	=2004BaltA..13..638C
by	COIA D. , McBREEN B., METCALFE L., BIVIANO A., ALTIERI B., MELLIER Y., OTT S., KNEIB J.P., O'HALLORAN B.
	Baltic Astronomy, 13, 638-641 (2004)
	Luminous infrared galaxies in the cluster Cl 0024+1654.
o	Fig.1: <[CMM2004] NN> (Nos 1-19, 22-46).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMM2005]
[CMM2005]	(Coia+Metcalfe+McBreen+, 2005)
Write:	<<[CMM2005] ISO-A2219-NN>> <<[CMM2005] A2219 A>>
N:	10+3
Object:	(Mid IR) + Arc (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	ISOCAM survey of ACO 2219. See also [BAH99] and [BGB2004]. N=10 Mid-IR sources are found. N=2 lensing arcs A and B. 'C' is the second brightest cluster member.
in source:	ACO 2219
Ref:	=2005A&A...430...59C
by	COIA D. , METCALFE L., McBREEN B., BIVIANO A., SMAIL I., ALTIERI B., KNEIB J.-P., McBREEN S., SANCHEZ-FERNANDEZ C., O'HALLORAN B.
	Astron. Astrophys., 430, 59-66 (2005)
	An ISOCAM survey through gravitationally lensing galaxy clusters. III. New results from mid-infrared observations of the cluster Abell 2219.
o	Table 2, Fig.1: <[CMM2005] ISO-A2219-NN> (Nos 1 to 10). Fig.1: <[CMM2005] A2219 A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMM2017]
[CMM2017]	(Carniani+Marconi+Maiolino+, 2017)
Write:	<<[CMM2017] LBQS0109-A>> <<[CMM2017] HB8903-A>> <<[CMM2017] 2QZJ0028-A>>
N:	3+2+1
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	ALMA 3mm observations of N=3+2+1 sources in the field of three quasars.
Ref:	=2017A&A...605A.105C
by	CARNIANI S. , MARCONI A., MAIOLINO R., FERUGLIO C., BRUSA M., CRESCI G., CANO-DIAZ M., CICONE C., BALMAVERDE B., FIORE F., FERRARA A., GALLERANI S., LA FRANCA F., MAINIERI V., MANNUCCI F., NETZER H., PICONCELLI E., SANI E., SCHNEIDER R., SHEMMER O., TESTI L.
	Astron. Astrophys., 605A, 105-105 (2017)
	AGN feedback on molecular gas reservoirs in quasars at z ~ 2.4.
o	Figs A.1+A.2+A.5, Table A.1: <[CMM2017] LBQS0109-A> (Nos A-C), <[CMM2017] HB8903-A> (Nos A-B), <[CMM2017] 2QZJ0028-A> (No. A).
o	CID-947 is XMMC 60131 in SIMBAD
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMN2008]
[CMN2008]	(Clark+Muno+Negueruela+, 2008)= (C07)
Write:	<<[CMN2008] JHHMMSS.s+DDMMSS>> <<[CMN2008] C07-XN>> <<[CMN2008] XN>> (not recognised by Simbad, but found in literature)
N:	241
Object:	(X) + * (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS-S observations of Cl Westerlund 1. N=241 X-ray point sources, among which N=7 new optical identifications are found.
in source:	Cl Westerlund 1
Ref:	=2008A&A...477..147C
by	CLARK J.S. , MUNO M.P., NEGUERUELA I., DOUGHERTY S.M., CROWTHER P.A., GOODWIN S.P., DE GRIJS R.
	Astron. Astrophys., 477, 147-163 (2008)
	Unveiling the X-ray point source population of the Young Massive Cluster Westerlund 1.
o	Table 1: <[CMN2008] JHHMMSS.s+DDMMSS> N=241. Table 3, col(5): <[CMN2008] C07-XN> (Nos X1 to X7).
=E=	Catalogue in electronic form as J/A+A/477/147
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMO99]
[CMO99]	(Cook+Mateo+Olszewski+, 1999)
Write:	<<[CMO99] CN>> <<[CMO99] KN>>
N:	1+3
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=1 C* (No. C1), and N=3 K giants (Nos K1-K3), in LGS 3.
in source:	LGS 3
Ref:	=1999PASP..111..306C
by	COOK K.H. , MATEO M., OLSZEWSKI E.W., VOGT S.S., STUBBS C., DIERCKS A.
	Publ. Astron. Soc. Pac., 111, 306-312 (1999)
	The systemic velocity and internal kinematics of the dwarf galaxy LGS 3: an optical foray beyond the Milky Way.
o	Fig. 2, GSC 01040+2152 is GSC 01195-0286.
o	Table 2: <[CMO99] C1> N=1, <[CMO99] KN> (Nos K1-K3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMP2004]
[CMP2004]	(Curran+Murphy+Pihlstrom+, 2004)
Write:	<<[CMP2004] QSO JHHMM+DDMM abs N.NNN>>
N:	4
Object:	DLA
Note:	Green Bank telescope and BIMA array are used to search for DLAs in QSOs line of sight. Among the 22 DLAs in Table 1, 18 are already known, see [SW2000b], [EPS2001], [EYH2001], [PGW2003] and [RKV2003]
Ref:	=2004MNRAS.352..563C
by	CURRAN S.J. , MURPHY M.T., PIHLSTROEM Y.M., WEBB J.K., BOLATTO A.D., BOWER G.C.
	Mon. Not. R. Astron. Soc., 352, 563-570 (2004)
	Molecular fraction limits in Damped Lyman Alpha Absorption systems.
o	Table 1: among the 22 DLAs, 18 are already known, see [SW2000b], [EPS2001], [EYH2001], [PGW2003] and [RKV2003]
o	Table 1: <[CMP2004] QSO J1024-0052 abs 2.398> N=1, <[CMP2004] QSO J1405+0415 abs N.NNN> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMP2007]
[CMP2007]	(Capalbi+Malesani+Perri+, 2007)
Write:	<<[CMP2007] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	SWift, X-ray observations of GRB 050408 field: discovery of a previously uncatalogued X-ry source.
Ref:	=2007A&A...462..913C
by	CAPALBI M. , MALESANI D., PERRI M., GIOMMI P., COVINO S., CUSUMANO G., MANGANO V., MINEO T., CAMPANA S., CHINCARINI G., LA PAROLA V., MORETTI A., ROMANO P., TAGLIAFERRI G., ANGELINI L., BOYD P., BURROWS D.N., GODET O., HILL J.E., KENNEA J.A., MARSHALL F., O'BRIEN P.T., GEHRELS N.
	Astron. Astrophys., 462, 913-918 (2007)
	Long-term monitoring of the X-ray afterglow of GRB 050408 with Swift/XRT.
o	Paragr. 2.1: <[CMP2007] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMP2009]
[CMP2009]	(Costa+Mendez+Pedreros+, 2009) (Not yet in Simbad)
Write:	<<[CMP2009] LMC QJHHMM+DDMM NN>> <<[CMP2009] SMC QJHHMM+DDMM NNN>>
N:	41+44
Object:	* (SIMBAD class: Star)
Note:	2.5m Du Pont telescope (Las Campanas Observatory, Chile) observations of the Magellanic Clouds to determiner their proper motion.
in source:	NAME Magellanic Clouds
in source:	Magellanic Clouds:LMC = LMC
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2009AJ....137.4339C
by	COSTA E. , MENDEZ R.A., PEDREROS M.H., MOYANO M., GALLART C., NOEL N., BAUME G., CARRARO G.
	Astron. J., 137, 4339-4360 (2009)
	The proper motion of the Magellanic clouds. I. First results and description of the program.
o	Table 3: <[CMP2009] LMC QJ0557-6713 NN> N=41 among (Nos 5-77). Table 4: <[CMP2009] SMC QJ0036-7227 NNN> N=44 among (Nos 12-286).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMP2012]
[CMP2012]	(Caramazza+Micela+Prisinzano+, 2012)
Write:	<<[CMP2012] NNNN>>
N:	1021
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS observations of N=1021 X-ray sources in NGC 1893.
in source:	NGC 1893
Ref:	=2012A&A...539A..74C
by	CARAMAZZA M. , MICELA G., PRISINZANO L., SCIORTINO S., DAMIANI F., FAVATA F., STAUFFER J.R., VALLENARI A., WOLK S.J.
	Astron. Astrophys., 539A, 74-74 (2012)
	Star formation in the Outer galaxy: coronal properties of NGC 1893.
o	Table 1: <[CMP2012] NNNN> (Nos 1-1021).
=E=	Catalogue in electronic form as J/A+A/539/A74
Details on Acronym: [CMR2006]
[CMR2006]	(Colbert+Malkan+Rich, 2006)
Write:	<<[CMR2006] HHMM+DDd ANNN>> <<[CMR2006] JHHMM+DDd ANNN>> <<[CMR2006] JHHMM+DDMM ANNN>> <<[CMR2006] HHMM+DDd ANNN>> (not recognised by Simbad, but found in literature) <<[CMR2006] HHMM+DDMM ANNN>> <<[CMR2006] HHMM ANNN>> <<[CMR2006] HHMM ANNN>>
N:	146+24
Object:	G + * (SIMBAD class: Galaxy)
Note:	Bright Age Survey over 6 separate fields. Keck LRIS observations of NIR sources.
Ref:	=2006ApJ...648..250C
by	COLBERT J.W. , MALKAN M.A., RICH R.M.
	Astrophys. J., 648, 250-267 (2006)
	The Bright Ages Survey. II. Evolution of luminosity, dust extinction, and star formation from z=0.5 to z=2.5.
o	Table 2: <[CMR2006] HHMM+DDd ANNN>, <[CMR2006] JHHMM+DDd ANNN>, <[CMR2006] JHHMM+DDMM ANNN>, N=146+24.
=E=	Catalogue in electronic form as J/ApJ/648/250
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMR2007]
[CMR2007]	(Cortese+Marcillac+Richard+, 2007)
Write:	<<[CMR2007] JHHMMSS+DDMMSS>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 and ACS, VLT ISAAC, Spitzer MIPS and IRAC observations of N=2 peculiar galaxies falling into the galaxy clusters Abell 1689 and Abell 2667, respectively.
in source:	ACO 1689
in source:	ACO 2667
Ref:	=2007MNRAS.376..157C
by	CORTESE L. , MARCILLAC D., RICHARD J., BRAVO-ALFARO H., KNEIB J.-P., RIEKE G., COVONE G., EGAMI E., RIGBY J., CZOSKE O., DAVIES J.
	Mon. Not. R. Astron. Soc., 376, 157-172 (2007)
	The strong transformation of spiral galaxies infalling into massive clusters at z ~ 0.2.
o	Figs 1-2, Table 1: <[CMR2007] JHHMMSS+DDMMSS> N=2.
o	Galaxy 131124-012040 = [GH91] 21, Galaxy 235144-260358 = APMUKS (BJ) B234908.95-262039.7
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CMS
CMS	(Campana+Mereghetti+Sidoli)
Write:	<<CMS NN>>
N:	33
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations N=33 stars in the field of RX J1856.5-3754. See also [W2001] and WWN.
Ref:	=1997A&A...320..783C
by	CAMPANA S. , MEREGHETTI S., SIDOLI L.
	Astron. Astrophys., 320, 783-786 (1997)
	Is RX J1856.5-3754 an old neutron star?
o	Table 1: <CMS NN> (Nos 1-33)
Origin	of the Acronym: L (1997A&A...318L..43N)
Details on Acronym: [CMS2002]
[CMS2002]	(Clements+McDowell+Shaked+, 2002)
Write:	<<[CMS2002] X-N>> <<[CMS2002] X-1 halo>>
N:	4+1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of APG 220.
in source:	IC 4553 = APG 220
Ref:	=2002ApJ...581..974C
by	CLEMENTS D.L. , McDOWELL J.C., SHAKED S., BAKER A.C., BORNE K., COLINA L., LAMB S.A., MUNDELL C.
	Astrophys. J., 581, 974-980 (2002)
	Chandra observations of Arp 220: the nuclear source.
o	Table 1: <[CMS2002] X-N> (Nos X-1 to X-4), <[CMS2002] X-1 halo> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMS2003]
[CMS2003]	(Clocchiatti+Minitti+SpuperMACHO+, 2003)
Write:	<<[CMS2003] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	Discovery of a new QSO.
Ref:	=2003IAUC.8258....1C
by	CLOCCHIATTI A. , MINITTI D., (The SuperMACHO Project), AGUILERA C., BECKER A., COOK K., COVARRUBIAS R., HAWLEY S., HIRIART R., KELLER S., MICELI A., MIKNAITIS G., NIKOLAEV S., OLSEN K., PRIETO J., PROCTOR G., REST A., SCHMIDT B., SMITH C., STUBBS C., SUNTZEFF N., WELCH D.
	IAU Circ., 8258, 1-None (2003)
	Quasar outburst in Mensa.
o	<[CMS2003] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMS2006]
[CMS2006]	(Cypriano+Mendes de Oliveira+Sodre, 2006)
Write:	<<[CMS2006] GSS.s+MMSS>>
N:	54
Object:	G + G in ClG (SIMBAD class: Galaxy)
Note:	Spectrographic observations with GMOS on the Gemini North Telescope of the fossil cluster RX J1416.4+2315. Format based on J2000.0 coordinates: complete coordinates are 14h 16m SS.s +23deg MM SS.
Ref:	=2006AJ....132..514C
by	CYPRIANO E.S. , MENDES DE OLIVEIRA C.L., SODRE L.Jr
	Astron. J., 132, 514-520 (2006)
	Velocity dispersion, mass, and the luminosity function of the fossil cluster RX J1416.4+2315.
o	Table 1: <[CMS2006] GSS.s+MMSS> N=54.
=E=	Catalogue in electronic form as J/AJ/132/514
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMS2009]
[CMS2009]	(Cersosimo+Mader+Santiago Figueroa+, 2009)
Write:	<<[CMS2009] GLLL.lll-BB.bbb>>
N:	13
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Parkes multibeam observations at the H166alpha line frequency (1424.734MHz).
Ref:	=2009ApJ...699..469C
by	CERSOSIMO J.C. , MADER S., SANTIAGO FIGUEROA N., FIGUEROA VELEZ S., SOTO C.L., AZCARATE D.
	Astrophys. J., 699, 469-477 (2009)
	Warped ionized hydrogen in the galaxy.
o	Tables 1-2: <[CMS2009] GLLL.lll-BB.bbb> N=13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMS2011]
[CMS2011]	(Capak+Mobasher+Scoville+, 2011)
Write:	<<[CMS2011] N>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Subaru, CFHT, and UKIRT observations of the COSMOS field. N=7 z>7 galaxy candidates.
Ref:	=2011ApJ...730...68C
by	CAPAK P. , MOBASHER B., SCOVILLE N.Z., McCRACKEN H., ILBERT O., SALVATO M., MENENDEZ-DELMESTRE K., AUSSEL H., CARILLI C., CIVANO F., ELVIS M., GIAVALISCO M., JULLO E., KARTALTEPE J., LEAUTHAUD A., KOEKEMOER A.M., KNEIB J.-P., LE FLOCH E., SANDERS D.B., SCHINNERER E., SHIOYA Y., SHOPBELL P., TANAGUCHI Y., THOMPSON D., WILLOTT C.J.
	Astrophys. J., 730, 68 (2011)
	Spectroscopy of luminous z > 7 galaxy candidates and sources of contamination in z > 7 galaxy searches.
o	Table 1: <[CMS2011] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMS2015]
[CMS2015]	(Coppola+Marconi+Stetson+, 2015)
Write:	<<[CMS2015] NNN>>
N:	101
Object:	SX* (SIMBAD class: SXPheV* = SX Phe Variable)
Note:	CTIO 4m and 1.5m telescopes, ASO 3.6m NTT, MPI/ESO 2.2m telescope, and ESO VLT observations of N=101 SX Phe variable stars in the Carina dwarf spheroidal galaxy. See also [VM2013].
in source:	NAME Carina Dwarf Galaxy
Ref:	=2015ApJ...814...71C
by	COPPOLA G. , MARCONI M., STETSON P.B., BONO G., BRAGA V.F., RIPEPI V., DALL'ORA M., MUSELLA I., BUONANNO R., FABRIZIO M., FERRARO I., FIORENTINO G., IANNICOLA G., MONELLI M., NONINO M., THEVENIN F., WALKER A.R.
	Astrophys. J., 814, 71 (2015)
	The Carina project IX: on hydrogen and helium burning variables.
o	Table 2: <[SMS86] NNN> (Nos 208-237) added. Table 12: <[CMS2015] NNN> (Nos 341-442).
=E=	Catalogue in electronic form as <J/ApJ/814/71/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMS84]
[CMS84]	(Carswell+Morton+Smith+, 111984)
Write:	<<[CMS84] N>>
N:	5 among 9
Object:	G (SIMBAD class: Galaxy)
Note:	N=5 galaxies among (Nos 1-9), in the field of QSO 1101-264 Map in Plate 4
Ref:	=1984ApJ...278..486C
by	CARSWELL R.F. , MORTON D.C., SMITH M.G., STOCKTON A.N., TURNSHEK D.A., WEYMANN R.J.
	Astrophys. J., 278, 486-498 (1984)
	The absorption line profiles in Q 1101-264.
o	Table 5: <[CMS84] N> N=5 among (Nos 2-9)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMV2003]
[CMV2003]	(Centurion+Molaro+Vladilo+, 2003)
Write:	<<[CMV2003] QSO JHHMM+DDMM abs N.NNN>>
N:	1+2
Object:	DLA
Note:	Observations of DLAs in the line of sight of QSOs. Among the DLAs cited in this paper, only 3 are not already known under an other acronym.
Ref:	=2003A&A...403...55C
by	CENTURION M. , MOLARO P., VLADILO G., PEROUX C., LEVSHAKOV S.A., D'ODORICO V.
	Astron. Astrophys., 403, 55-72 (2003)
	Early stages of nitrogen enrichment in galaxies: Clues from measurements in damped Lyman α systems.
o	Table 9: QXO 0001 not identified.
o	Tables 1, 9: <[CMV2003] QSO JHHMM+DDMM abs N.NNN> N=1+2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMV96]
[CMV96]	(Chambers+Miley+Van Breugel+, 1996)
Write:	<<[CMV96] 4C DDNNAA>> <<[CMV96] 4C DD.NNW>> <<[CMV96] 4C DD.NN AN>>
N:	163
Object:	(Rad) + * (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Objects with a format '4C DDNNAA' are stars (This format is only 'DDNNAA' in the table 3 of the 1st ref. and the table 1 of the 2nd ref.). The format is constructed on the 4C DD.NN associated with the star N=26 (1st ref. T.3) and N=15+2 (2nd ref. T.1 and 2) The object 4C 26.38 is two different sources North and South, '[CMV96] 4C 26.38N' and [CMV96] 4C 26.38S' The sources 4C DD.NN have components, format '4C DD.NN AN' N=83 (1st ref. T.4) and N=53 (2nd ref. T.2) Maps
Ref:	=1996ApJS..106..215C
by	CHAMBERS K.C. , MILEY G.K., VAN BREUGEL W.J.M., HUANG J.-S.
	Astrophys. J., Suppl. Ser., 106, 215-246 (1996)
	Ultra-Steep-Spectrum radio sources. I. 4C Objects.
o	Table 3: the format 'DDNNA' is '4C DDNNA' in SIMBAD
o	Table 1: <[CMV96] 4C 26.38W> N=2. Table 3: <[CMV96] 4C DDNNAA> N=26. Table 4: <[CMV96] 4C DD.NN AN> N=83
Ref:	=1996ApJS..106..247C
by	CHAMBERS K.C. , MILEY G.K., VAN BREUGEL W.J.M., BREMER M.A.R., HUANG J.-S., TRENTHAM N.A.
	Astrophys. J., Suppl. Ser., 106, 247-280 (1996)
	Ultra-Steep-Spectrum radio sources. II. Radio, infrared, optical, and HST imaging of high-redshift 4C objects.
o	Tables 1, 2: the format 'DDNNA' is '4C DDNNA' in SIMBAD
o	Tables 1, 2: <[CMV96] 4C DDNNAA> N=15+2. Table 2: <[CMV96] 4C DD.NN AN> N=53
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMW2000]
[CMW2000]	(Caretta+Maia+Willmer, 2000)= ([CMW2000a])
Write:	<<[CMW2000] 5-NN>> <<[CMW2000] 7-N>>
N:	15+5
Object:	G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Objects classified as G and or Star in PDS (Photometric Data System) and in SSC (Southern Sky Catalog). Table 5 (first digit in the format): (Nos 1-5) are G in both catalogs, (Nos 6-10) are G in PDS and * in SSC, (Nos 11-15) are stars in both catalogs. Map in Fig.4. Table 7 (first digit in the format): (Nos 1-5) are G in PDS and * in SSC. Map in Fig.8.
Ref:	=2000AJ....119..524C
by	CARETTA C.A. , MAIA M.A.G., WILLMER C.N.A.
	Astron. J., 119, 524-535 (2000)
	A quantitative evaluation of the galaxy component of the COSMOS and APM catalogs.
o	Table 5: <[CMW2000] 5-NN> (Nos 5-1 to 5-15). Table 7: <[CMW2000] 7-N> (Nos 7-1 to 7-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMW2000a]
[CMW2000a]	(Caretta+Maia+Willmer, 2000)
*****	Avoid the usage of [CMW2000a], prefer [CMW2000]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMW2000b]
[CMW2000b]	(Colafrancesco+Mullis+Wolter+, 2000)
Write:	<<[CMW2000b] A>> <<[CMW2000b] gN>>
N:	4+5
Object:	AGN + * + G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	UH and Keck observations. Table 2, Fig.3: (Nos A-D), 4 objects in the field of 1SAX J0027.1-1926 and 1SAX J0027.0-1928. No. A is an AGN, No. B is a star, Nos C and D are galaxies. (Nos g1-g5), 5 galaxies in the field of 1SAX J0027.2-1930.
Ref:	=2000A&AS..144..187C
by	COLAFRANCESCO S. , MULLIS C.R., WOLTER A., GIOIA I.M., MACCACARO T., ANTONELLI A., FIORE F., KAASTRA J., MEWE R., REPHAELI Y., FUSCO-FEMIANO R., ANTONUCCIO-DELOGU V., MATTEUCCI F., MAZZOTTA P.
	Astron. Astrophys., Suppl. Ser., 144, 187-194 (2000)
	An X-ray and optical study of the cluster A33.
o	Table 2, Fig.3: <[CMW2000b] A> (Nos A-D), <[CMW2000b] gN> (Nos g1-g5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CMW2004]
[CMW2004]	(Caretta+Maia+Willmer, 2004)
Write:	<<[CMW2004] NNN>>
N:	920
Object:	G (SIMBAD class: Galaxy)
Note:	Catalog of 920 galaxies selected in 68 fields of the Aquarius Cluster Catalog. See also Paper I: AqrCC.
Ref:	=2004AJ....128.2642C
by	CARETTA C.A. , MAIA M.A.G., WILLMER C.N.A.
	Astron. J., 128, 2642-2651 (2004)
	The Aquarius superclusters. II. Spectroscopic and photometric data.
o	Table 5: <[CMW2004] NNN> (Nos 1-920).
=E=	Catalogue in electronic form as J/AJ/128/2642
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CN
CN	(Couch+Newell)= (CN84)
Write:	<<CN ANNNN NNN>> <<CN ACNNN NNNA>> <<CN CHHMM+DD NNN>>
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	In numerous references, the authors refers as 'CN' a survey of Couch + Newell in several ClG, never completely published. The galaxies are 'CN' cross-identified with another acronym with the same format in SIMBAD: [CEG83], [CN84], [ECM85], [CS87], [MEC88]
in source:	ACO 370
in source:	ACO 1525
in source:	ACO 1689
in source:	ACO 1942
in source:	ACCG 103 = ACO S 910
in source:	ACCG 106 = ACO 3665
in source:	ACCG 113 = ACO 3934
in source:	ACCG 114 = ACO S 1077
in source:	ACCG 116 = ACO 4041
in source:	ACCG 118 = ACO 2744
in source:	ACCG 121 = ACO 3157
in source:	ACCG 122 = ACO 3207
in source:	ClG 0016+1609 = 1E 0015.9+1609
Ref:	=1983MNRAS.205.1287C
by	COUCH W.J. , ELLIS R.S., GODWIN J., CARTER D.
	Mon. Not. R. Astron. Soc., 205, 1287-1312 (1983)
	Spectral energy distributions for galaxies in high redshift clusters - I. Methods and application to three clusters with 0.22 < z < 0.31.
o	Plates 1a, 1b, 1c: <[CEG83] A1942 NN> = <CN A1942 NN> Nos among (Nos 1-81), <[CEG83] A1525 NN> = <CN A1525 NN> Nos among (Nos 1-62), <[CEG83] AC103 NNN> = <CN AC103 NNN> Nos among (Nos 1-145).
Ref:	=1984ApJS...56..143C
by	COUCH W.J. , NEWELL E.B.
	Astrophys. J., Suppl. Ser., 56, 143-192 (1984)
	Distant clusters of galaxies. I. Uniform photometry of 14 rich clusters.
o	Table 2: <[CN84] ACCG NNN N> = <CN ACNNN N>, <[CN84] ACO NNNN NN> = <CN ANNNN N>, N=32.
Ref:	=1985MNRAS.217..239E
by	ELLIS R.S. , COUCH W.J., MacLAREN I., KOO D.C.
	Mon. Not. R. Astron. Soc., 217, 239-264 (1985)
	Spectral energy distributions for galaxies in high-redshift clusters - II. 0016+16 at z = 0.54.
o	Table 5: <[ECM85] NNN> = <CN C0016+16 NNN>, N=47 among 150.
Ref:	=1987MNRAS.229..423C
by	COUCH W.J. , SHARPLES R.M.
	Mon. Not. R. Astron. Soc., 229, 423-456 (1987)
	A spectroscopic study of three rich galaxy clusters at ζ=0.31.
o	Table 2: <[CS87] AC103 NNN> = <CN AC103 NNN> N=60 among 430. Table 3: <[CS87] AC114 NNN> = <CN AC114 NNN> N=52 among 859. Table 4: <[CS87] AC118 NNN> = <CN AC118 NNN> N=40 among 398.
Ref:	=1988MNRAS.230..249M
by	MacLAREN I. , ELLIS R.S., COUCH W.J.
	Mon. Not. R. Astron. Soc., 230, 249-272 (1988)
	Spectral energy distributions of galaxies in high-redshift clusters. III. Abell 370 at z=0.37.
o	Table 3: <[MEC88] NNN> = <CN A370 NNN> N=124 among (Nos 1-297).
Ref:	=1994ApJ...430..121C
by	COUCH W.J. , ELLIS R.S., SHARPLES R.M., SMAIL I.
	Astrophys. J., 430, 121-138 (1994)
	Morphological studies of the galaxy populations in distant "Butcher-Oemler" clusters with HST. I. AC 114 at z = 0.31 and Abell 370 at z = 0.37.
o	Tables 2, 3, 4: <[CS87] AC114 NNN> = <CN AC114 NNN> Nos among (Nos 30-832).
Origin	of the Acronym: L (1988MNRAS.230..249M,1987MNRAS.229..423C,1998ApJ...497..188C)
Details on Acronym: CN
CN	(Cometary Nebula)
*****	Avoid the usage of CN, prefer [MKM2003b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cn
Cn	(Cannon)
Write:	<<PN Cn 1-N>> <<PN Cn 2-N>> <<PN Cn 3-N>>
N:	6+1+1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	List 1: format '1-N', N=6. List 2: Cn 2-1 = PN G356.2-04.4 = PK 356-4 1. List 3: Cn 3-1 = PN G038.2+12.0 = PK 038+12 1.
Ref:	=1921HarCi.224....1C
by	CANNON A.J.
	Harvard Circ., 224, 1-None (1921)
	Stars having peculiar spectra. 16 new variable stars.
o	<PN Cn 1-N> N=6
Ref:	=1923BHarO.784....1C
by	CANNON A.J.
	Harvard Bull., 784, 1-None (1923)
	New planetary nebula.
o	<PN Cn 2-N> (No. 2-1).
Ref:	=1926BHarO.837....2C
by	CANNON A.J.
	Harvard Bull., 837, 2-None (1926)
	Peculiar spectra.
o	<PN Cn 3-N> (No. 3-1).
Details on Acronym: CN84
CN84	(Couch+Newell, 1984)
*****	Avoid the usage of CN84, prefer CN
Origin	of the Acronym: L (2006ApJ...644..116M)
Details on Acronym: [CN84]
[CN84]	(Couch+Newell, 1984)= (CN)
Write:	<<[CN84] ACCG NNN N>> <<[CN84] ACO NNNN NN>>
N:	32
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table 2: G in ACCG or ACO cluster of G. Maps in Fig. 15 See also CN
in source:	ACO 370
in source:	ACO 1525
in source:	ACO 1689
in source:	ACCG 106 = ACO 3665
in source:	ACCG 103 = ACO S 910
in source:	ACCG 113 = ACO 3934
in source:	ACCG 114 = ACO S 1077
in source:	ACCG 116 = ACO 4041
in source:	ACCG 118 = ACO 2744
in source:	ACCG 121 = ACO 3157
in source:	ACCG 122 = ACO 3207
Ref:	=1984ApJS...56..143C
by	COUCH W.J. , NEWELL E.B.
	Astrophys. J., Suppl. Ser., 56, 143-192 (1984)
	Distant clusters of galaxies. I. Uniform photometry of 14 rich clusters.
o	Table 2: <[CN84] ACCG NNN N> = <CN ACNNN N>, <[CN84] ACO NNNN NN> = <CN ANNNN N>, N=32.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CNA2008]
[CNA2008]	(Cappa+Niemela+Amorin+, 2008)
Write:	<<[CNA2008] NN>>
N:	47
Object:	Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Note:	Search for YSO candidates in Gum 31 HII region in the IRAS, 2MASS and MSX6C catalogs.
in source:	GUM 31
Ref:	=2008A&A...477..173C
by	CAPPA C. , NIEMELA V.S., AMORIN R., VASQUEZ J.
	Astron. Astrophys., 477, 173-183 (2008)
	The environs of the H II region Gum31.
o	Table 3: <[CNA2008] NN> (Nos 1-47).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CNC2015]
[CNC2015]	(Chen+Nurnberger+Chini+, 2015)
Write:	<<[CNC2015] B273A>> <<[CNC2015] IRS5A>>
N:	2+5
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	VLT NACO AO observations of the hypercompact HII M17 UC1.
in source:	Cl* NGC 6618 B 273
in source:	[CW98] IRS 5
Ref:	=2015A&A...578A..82C
by	CHEN Z. , NUERNBERGER D.E.A., CHINI R., JIANG Z., FANG M.
	Astron. Astrophys., 578A, 82-82 (2015)
	VLT near- to mid-IR imaging and spectroscopy of the M17 UC1-IRS5 region.
o	Fig. 1, Table 2: <[CNC2015] B273A> (Nos B273A-B273B), <[CNC2015] IRS5A> (Nos IRS5A-IRS5E).
Details on Acronym: [CND2009]
[CND2009]
Write:	<<[CND2009] SNN>>
N:	28
Object:	* (SIMBAD class: Star)
Note:	AZT-24 1.1m telescope SWIRCAM and UKIRT UIST spectroscopic observations of the red supergiante dominated cluster RSGC 3.
in source:	RSGC 3
Ref:	=2009A&A...498..109C
by	CLARK J.S. , NEGUERUELA I., DAVIES B., LARIONOV V.M., RITCHIE B.W., FIGER D.F., MESSINEO M., CROWTHER P.A., ARKHAROV A.A.
	Astron. Astrophys., 498, 109-114 (2009)
	A third red supergiant rich cluster in the Scutum-Crux arm.
o	Paragraph 4. RSCG 3 (group of galaxies) is a probable misprint for RSGC 3 (cluster of stars).
o	Text: <RSGC N> (No. 3) added. Table 1: <[CND2009] SNN> (Nos S1-S28).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CND2015]
[CND2015]	(Collet+Nesvadba+De Breuck+, 2015)
Write:	<<[CND2015] a>>
N:	7
Object:	Poss. G (SIMBAD class: Galaxy_Candidate = Galaxy Candidate)
Note:	VLT ISAAC observations of N=7 Hα candidates around TXS 2353-003.
Ref:	=2015A&A...579A..89C
by	COLLET C. , NESVADBA N.P.H., DE BREUCK C., LEHNERT M.D., BEST P., BRYANT J.J., DICKEN D., JOHNSTON H., HUNSTEAD R., WYLEZALEK D.
	Astron. Astrophys., 579A, 89-89 (2015)
	Defying jet-gas alignment in two radio galaxies at z ~ 2 with extended light profiles: Similarities to brightest cluster galaxies.
o	Table 2: <[CND2015] a> N=7 (Nos a-g).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CNG2015]
[CNG2015]	(Canameras+Nesvadba+Guery+, 2015)
Write:	<<[CNG2015] PLCK GLLL.l+BB.b>>
N:	11
Object:	Grav. lensed image of a G (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	IRAM 30m telescope EMIR CO line observations of N=11 bright far-infrared (FIR) and sub-mm sources discovered through a combination of the Planck all-sky survey and follow-up Herschel-SPIRE imaging, also known as "Planck’s Dusty GEMS (Gravitationally Enhanced subMillimetre Sources)". Use of SDSS data.
Ref:	=2015A&A...581A.105C
by	CANAMERAS R. , NESVADBA N.P.H., GUERY D., McKENZIE T., KOENIG S., PETITPAS G., DOLE H., FRYE B., FLORES-CACHO I., MONTIER L., NEGRELLO M., BEELEN A., BOONE F., DICKEN D., LAGACHE G., LE FLOC'H E., ALTIERI B., BETHERMIN M., CHARY R., DE ZOTTI G., GIARD M., KNEISSL R., KRIPS M., MALHOTRA S., MARTINACHE C., OMONT A., POINTECOUTEAU E., PUGET J.-L., SCOTT D., SOUCAIL G., VALTCHANOV I., WELIKALA N., YAN L.
	Astron. Astrophys., 581A, 105-105 (2015)
	Planck's dusty GEMS: The brightest gravitationally lensed galaxies discovered with the Planck all-sky survey.
o	Table 1: <[CNG2015] PLCK GLLL.l+BB.b> N=11.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CNK2017]
[CNK2017]	(Canameras+Nesvadba+Kneissl+, 2017)
Write:	<<[CNK2017] PLCK G244.8+54.9 system>> <<[CNK2017] PLCK G244.8+54.9 lens>> <<[CNK2017] PLCK G244.8+54.9 N.N>>
N:	1+1+6
Object:	Grav. lens system + Grav. lens + Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2, HAWK-I and XShooter, and ALMA Band 3 observations of N=1 gravitational lens and N=6 gravitationally lensed images of the background galaxy [CNG2015] PLCK G244.8+54.9, forming N=1 gravitational lens system. See also [CNL2018].
Ref:	=2017A&A...600L...3C
by	CANAMERAS R. , NESVADBA N.P.H., KNEISSL R., LIMOUSIN M., GAVAZZI R., SCOTT D., DOLE H., FRYE B., KOENIG S., LE FLOC'H E., OTEO I.
	Astron. Astrophys., 600L, 3-3 (2017)
	Planck's dusty GEMS. III. A massive lensing galaxy with a bottom-heavy stellar initial mass function at z = 1.5.
o	<[CNK2017] PLCK G244.8+54.9 system> N=1. <[CNK2017] PLCK G244.8+54.9 lens> N=1. Fig. 3: <[CNK2017] PLCK G244.8+54.9 N.N> (Nos 1.1-1.4, 2.1-2.2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CNK98]
[CNK98]	(Comeron+Neuhauser+Kass, 1998)= (IR)
Write:	<<[CNK98] IR N>>
N:	3
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	ISOCAM observations of the centre of Vha I aggregate.
in source:	NAME Cha I
Ref:	=1998Msngr..94...28C
by	COMERON F. , NEUHAEUSER R., KAAS A.A.
	The Messenger, 94, 28-31 (1998)
	The first X-ray emitting brown dwarf.
o	Object B34 = BYB 34
o	Fig.2: <[CNK98] IR N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CNL2018]
[CNL2018]	(Canameras+Nesvadba+Limousin+, 2018)
Write:	<<[CNL2018] PLCK G165.7+67.0 system>> <<[CNL2018] PLCK G165.7+67.0 lens>> <<[CNL2018] PLCK G165.7+67.0 N.N>> <<[CNL2018] PLCK G165.7+67.0 Co-W>>
N:	1+1+24+2
Object:	Grav. lens system + Grav. lens + Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST WFC3, CFHT Megacam and WIRCAM, Spitzer IRAC, SMA and PdBI observations of N=1 gravitational lens, N=24+2 gravitationally lensed images of the background galaxy [CNG2015] PLCK G165.7+67.0, forming N=1 gravitational lens system. See also [CNK2017].
Ref:	=2018A&A...620A..60C
by	CANAMERAS R. , NESVADBA N.P.H., LIMOUSIN M., DOLE H., KNEISSL R., KOENIG S., LE FLOC'H E., PETITPAS G., SCOTT D.
	Astron. Astrophys., 620A, 60-60 (2018)
	Planck's dusty GEMS. V. Molecular wind and clump stability in a strongly lensed star-forming galaxy at z = 2.2.
o	<[CNL2018] PLCK G165.7+67.0 system> N=1. <[CNL2018] PLCK G165.7+67.0 lens> N=1. Fig. 5, Table 3: <[CNL2018] PLCK G165.7+67.0 N.N>, N=24 among (Nos 1.1-1.2 to 9.1-9.2). Figs 5+11, Table 6: <[CNL2018] PLCK G165.7+67.0 Co-W> (Nos Co-N, Co-S).
o	PLCK G165.7+49.0 is a misprint for [CNG2015] PLCK G165.7+67.0
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CNM2001]
[CNM2001]	(Castander+Nichol+Merrelli+, 2001)
Write:	<<[CNM2001] NNN>>
N:	196
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	SLOAN digital sky survey.
in source:	Coma Cluster = ACO 1656
Ref:	=2001AJ....121.2331C
by	CASTANDER F.J. , NICHOL R.C., MERRELLI A., BURLES S., POPE A., CONNOLLY A.J., UOMOTO A., GUNN J.E., ANDERSON J.E., ANNIS J., BAHCALL N.A., BOROSKI W.N., BRINKMANN J., CAREY L., CROCKER J.H., CSABAI I., DOI M., FRIEMAN J.A., FUKUGITA M., FRIEDMAN S.D., HILTON E.J., HINDSLEY R.B., IVEZIC Z., KENT S., LAMB D.Q., LEGER R.F., LONG D.C., LOVEDAY J., LUPTON R.H., MacGILLIVRAY H., MEIKSIN A., MUNN J.A., NEWCOMB M., OKAMURA S., OWEN R., PIER J.R., ROCKOSI C.M., SCHLEGEL D.J., SCHNEIDER D.P., SEIGMUND W., SMEE S., SNIR Y., STARKMAN L., STOUGHTON C., SZOKOLY G.P., STUBBS C., SUBBARAO M., SZALAY A., THAKAR A.R., TREMONTI C., WADDELL P., YANNY B., YORK D.G.
	Astron. J., 121, 2331-2357 (2001)
	The first hour of extragalactic data of the Sloan Digital Sky Survey spectroscopic commissioning: the Coma cluster.
o	Table 1: <[CNM2001] NNN> N=196 among (Nos 3-312).
=E=	Catalogue in electronic form as J/AJ/121/2331
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CnMy
CnMy	(Cannon+Mayall)
Write:	<<PN CnMy NN>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	= CnMy 17 = PK 001-06 1 PN excerpted from a list of 21 objects, rejected as a PN in 1992, Acker+ catalog
Ref:	=1938BHarO.908...20C
by	CANNON A.J. , MAYALL M.W.
	Harvard Bull., 908, 20-21 (1938)
	New peculiar spectra.
o	<PN CnMy NN> (No. 17), N=1.
Details on Acronym: [CNN81]
[CNN81]	(Cannon+Niss+Norgaard-Nielsen, 1981)
Write:	<<[CNN81] CN>>
N:	2
Object:	Carbon * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	In the format the letter 'C' stands for Carbon star
in source:	NAME Carina Dwarf Galaxy
Ref:	=1981MNRAS.196p...1C
by	CANNON R.D. , NISS B., NORGAARD-NIELSEN H.U.
	Mon. Not. R. Astron. Soc., 196, part no 16, 1-None (1981)
	The discovery of two carbon stars in the Carina dwarf galaxy.
o	<[CNN81] CN> (Nos C1-C2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CNOC
CNOC	(Canadian Network for Observ. Cosmology)= (CNOC1) = (PPP)
Write:	<<CNOC ACO NNNN FFNNNN>> <<CNOC MS HHMM FFNNNN>>
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	1996ApJS..102..269Y gives the 16 clusters in the survey: ACO 2390 + 15 EMSS clusters (MS HHMM in the format) In the format 'FFNNNN', 1st digit 'F' denotes the field (Nos 1-5) 2nd digit 'F' indicates whether the object is observed in one field (F=0), or in an overlapping area from two fields (F= field number of the overlapping field). The last 4 digits 'NNNN' denote the object number within its own field. In some MS HHMM.m+DDMM the authors don't write the complete format, only the central field been observed. In such a case, In SIMBAD, we use the complete format '10NNNN'. See also CNOC2 survey.
in source:	ACO 2390
in source:	1E 1621.5+2640 = ClG 1621+2640
in source:	1E 0302.7+1658 = ClG 0302+1658
in source:	1E 1358.4+6245 = ClG 1358+6245
in source:	1E 1008.1-1224 = ClG 1008-1224
in source:	1E 1224.0+2007
in source:	1E 1512.0+3647
in source:	1E 0015.9+1609 = ClG 0016+1609
in source:	1E 0451.6-0305 = ClG 0451-0305
Ref:	=1996ApJS..102..289Y
by	YEE H.K.C. , ELLINGSON E., ABRAHAM R.G., GRAVEL P., CARLBERG R.G., SMECKER-HANE T.A., SCHADE D., RIGLER M.
	Astrophys. J., Suppl. Ser., 102, 289-308 (1996)
	The CNOC cluster redshift survey catalogs. II. Abell 2390.
o	Table 2: <CNOC ACO 2390 FFNNNN> N=542
Ref:	=1997ApJS..113....1E
by	ELLINGSON E. , YEE H.K.C., ABRAHAM R.G., MORRIS S.L., CARLBERG R.G., SMECKER-HANE T.A.
	Astrophys. J., Suppl. Ser., 113, 1-21 (1997)
	The CNOC cluster redshift survey catalogs. III. MS 1621.5+2640 and MS 0302.7+1658.
o	Table 3: Used the complete format '10NNNN' (always a 6 digits format)
o	Table 2: <CNOC MS 1621 FFNNNN> N=507. Table 3: <CNOC MS 0302 10NNNN> N=185.
Ref:	=1998ApJS..116..211Y
by	YEE H.K.C. , ELLINGSON E., MORRIS S.L., ABRAHAM R.G., CARLBERG R.G.
	Astrophys. J., Suppl. Ser., 116, 211-230 (1998)
	The CNOC cluster redshift survey catalogs.
o	Table 2: <CNOC MS 1358 NNNNNN> N=373. Table 3: <CNOC MS 1008 10NNNN> N=188.
Ref:	=1998ApJS..116..231A
by	ABRAHAM R.G. , YEE H.K.C., ELLINGSON E., CARLBERG R.G., GRAVEL P.
	Astrophys. J., Suppl. Ser., 116, 231-246 (1998)
	The CNOC cluster redshift survey catalogs. V. MS 1224.7+2007 and MS 1512.4+3647.
o	Table 2: <CNOC MS 1224 10NNNN> N=114. Table 3: <CNOC MS 1512 NNNNNN> N=352.
Ref:	=1998ApJS..116..247E
by	ELLINGSON E. , YEE H.K.C., ABRAHAM R.G., MORRIS S.L., CARLBERG R.G.
	Astrophys. J., Suppl. Ser., 116, 247-262 (1998)
	The CNOC cluster redshift survey catalogs. VI. MS 0015.9+1609 and MS 0451.5-0305.
o	Table 2: <CNOC MS 0015 10NNNN> N=280. Table 3: <CNOC MS 0451 10NNNN> N=202.
=E=	Catalogue in electronic form as J/ApJS/102/289
=E=	Catalogue in electronic form as J/ApJS/113/1
=E=	Catalogue in electronic form as J/ApJS/116/211
=E=	Catalogue in electronic form as J/ApJS/116/231
=E=	Catalogue in electronic form as J/ApJS/116/247
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CNOC1
CNOC1	(Canadian Network for Observ. Cosmology, 1st catalog)
*****	Avoid the usage of CNOC1, prefer CNOC
Origin	of the Acronym: L (1997ApJ...475...29P)
Details on Acronym: CNOC2
CNOC2	(Canadian Network for Observ. Cosmology, 2nd catalog)
Write:	<<CNOC2 HHMM NNNNNN>>
N:	24101
Object:	G (SIMBAD class: Galaxy)
Note:	Catalog of faint galaxies in different 'patches': CNOC 0223+00, 0920+37, 1447+09, 2148-05 (only HHMM in the format) See also CNOC survey.
Ref:	=2000ApJS..129..475Y
by	YEE H.K.C. , MORRIS S.L., LIN H., CARLBERG R.G., HALL P.B., SAWICKI M., PATTON D.R., WIRTH G.D., ELLINGSON E., SHEPHERD C.W.
	Astrophys. J., Suppl. Ser., 129, 475-492 (2000)
	The CNOC2 field galaxy redshift survey. I. The survey and the catalog for the patch CNOC 0223+00.
o	Table 6: <CNOC2 0223 NNNNNN> N=62.
=E=	Catalogue in electronic form as J/ApJS/129/475
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CNOC2XGG
CNOC2XGG	(CNOC2 X-ray Galaxy Group)
Write:	<<CNOC2XGG JHHMMSS+DDMM.m>>
N:	25
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	X-ray detected galaxy groups in the CNOC2 survey. See also [FCP2009].
Ref:	=2009ApJ...704..564F
by	FINOGUENOV A. , CONNELLY J.L., PARKER L.C., WILMAN D.J., MULCHAEY J.S., SAGLIA R.P., BALOGH M.L., BOWER R.G., McGEE S.L.
	Astrophys. J., 704, 564-575 (2009)
	The roadmap for unification in galaxy group selection. I. A search for extended X-ray emission in the CNOC2 survey.
o	Table 1: <[FCP2009] XHHhNN> (Nos X14h01-X14h09, X21h01-X21h16) = <CNOC2XGG JHHMMSS+DDMM.m> N=25.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CNP2009]
[CNP2009]	(Christensen+Noterdaeme+Petitjean+, 2009)
Write:	<<[CNP2009] QHHMM abs N.NNNN>> <<[CNP2009] QHHMM Na>>
N:	4+13
Object:	DLA + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT FORS1 observations of fields towards two SDSS QSOs.
Ref:	=2009A&A...505.1007C
by	CHRISTENSEN L. , NOTERDAEME P., PETITJEAN P., LEDOUX C., FYNBO J.P.U.
	Astron. Astrophys., 505, 1007-1016 (2009)
	Uncovering strong MgII absorbing galaxies. Imaging below the Lyman limit.
o	Table 1: <[CNP2009] QHHMM abs N.NNNN> N=4. Table 2: <[CNP2009] QHHMM Na> N=5+8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CNS2013]
[CNS2013]	(Carlhoff+Nguyen Luong+Schilke+, 2013)
Write:	<<[CNS2013] NN>>
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	IRAM 30-m telescope 13CO(2-1) and C18O(2-1) observations of N=29 molecular clouds in the W43 complex.
in source:	W 43
Ref:	=2013A&A...560A..24C
by	CARLHOFF P. , NGUYEN LUONG Q., SCHILKE P., MOTTE F., SCHNEIDER N., BEUTHER H., BONTEMPS S., HEITSCH F., HILL T., KRAMER C., OSSENKOPF V., SCHULLER F., SIMON R., WYROWSKI F.
	Astron. Astrophys., 560A, 24-24 (2013)
	Large scale IRAM 30m CO-observations in the giant molecular cloud complex W43.
o	Fig. E.1, Tables 1-3: <[CNS2013] NN> (Nos 1-29).
o	Paragraph 2. G34.3 not identified (incomplete format).
=E=	Catalogue in electronic form as <J/A+A/560/A24/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CNS5
CNS5	(Fifth Catalogue of Nearby Stars)
Write:	<<CNS5 NNNN>>
N:	about 6000
Object:	* + PM* + ** + LM* + BD* (SIMBAD class: Star)
Note:	The Fifth Catalogue of Nearby Stars (CNS5) aims to provide the most volume-complete sample of stars in the solar neighbourhood. The CNS5 is compiled based on trigonometric parallaxes from Gaia EDR3 and Hipparcos, and supplemented with astrometric data from Spitzer and ground-based surveys carried out in the infrared. The CNS5 catalogue is statistically complete down to 19.7 mag in G-band and 11.8 mag in W1-band absolute magnitudes, corresponding to a spectral type of L8. Continuous updates of observational data for nearby stars from all sources were collected and evaluated. For all known stars in the 25 pc sphere around the Sun, the best values of positions in space, velocities, and magnitudes in different filters are presented. Catalogue: https://dc.g-vo.org/CNS5
Notes:	We are working on the next edition of the CNS already - CNS6. Similar to CNS5, objects in the catalogue will have two sets of designations: CNS6 NNNN as well as Gliese-Jahreiß numbers in the format GJ NNNN for numbers assigned before the CNS5 and GJ 1NNNN for numbers assigned in the CNS5 or in the CNS6.
Ref:	=2023A&A...670A..19G
by	GOLOVIN A. , REFFERT S., JUST A., JORDAN S., VANI A., JAHREISS H.
	Astron. Astrophys., 670A, 19 (2023)
	The Fifth Catalogue of Nearby Stars (CNS5).
o	<CNS5 NNNN> (Nos 0-5930). LSW, Heidelberg University
=E=	Catalogue in electronic form as <J/A+A/670/A19/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CNSS
CNSS	(Caltech-NRAO Stripe 82 Survey)
Write:	<<CNSS JHHMMSS.s+DDMMSS>>
Object:	Radio(cm) (SIMBAD class: cmRad = Centimetric Radio Source)
Note:	Five-epoch survey of SDSS Stripe 82 with the Jansky VLA at 3 GHz. Angular resolution ∼2 arcsec. http://www.tauceti.caltech.edu/stripe82/ http://www.astro.caltech.edu/~kunal/projects/stripe82/ https://library.nrao.edu/proposals/?utf8=%E2%9C%93&search_field=all_fields&q=VLA%2F13B-370 CNSS Pilot (Paper I; Mooley et al. 2015a; ApJ, submitted) CNSS Data release (Paper IV; Mooley et al. 2015b; in prep)
Auth.:	Kunal Mooley California Institute of Technology
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CNUM
CNUM	(Catalog Number)
*****	Avoid the usage of CNUM, prefer C*
Origin	of the Acronym: L (1988A&A...203...51W,1988A&A...203...65W)
Details on Acronym: Co
Co	(Courtes) (Not yet in Simbad)
*****	Avoid the usage of Co, prefer [C51]
Origin	of the Acronym: L (1976A&AS...25...25D)
Details on Acronym: CO
CO	(CO molecular cloud)
Write:	<<CO LLL.ll+BB.bb>> <<CO +LLL.ll+BB.bb>>
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Rem:	Systematic designation
Details on Acronym: CO
CO	(CO)
*****	Avoid the usage of CO, prefer LMC-CO
Origin	of the Acronym: L (1988PASP..100..346H)
Details on Acronym: Co
Co	(Coalsack DCld)
*****	Avoid the usage of Co, prefer [VMF94]
Origin	of the Acronym: L (1999ApJS..123..233L)
Details on Acronym: CoA
CoA	(Corona Australis cloud)
*****	Avoid the usage of CoA, prefer [VMF2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [COA2000]
[COA2000]	(Chakraborty+Ojha+Anandarao+, 2000)
Write:	<<[COA2000] NN>>
N:	12
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=12 stars toward IRAS 05361+3539. The numbering corresponds to SW2002 Star 1 to 12.
Ref:	=2000A&A...364..683C
by	CHAKRABORTY A. , OJHA D.K., ANANDARAO B.G., RENGARAJAN T.N.
	Astron. Astrophys., 364, 683-688 (2000)
	Massive and luminous YSO IRAS 05361+3539 and its environment. A study of star formation in the parent cloud - I.
o	Table 1: <[COA2000] NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [COA2012]
[COA2012]	(Carrasco-Gonzalez+Osorio+Anglada+, 2012)
Write:	<<[COA2012] IRS 2A>>
N:	2
Object:	(Rad) + YSO (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 3.6cm and CARMA 6cm observations of N=2 YSOs, components of the binary system [WRA93] IRS 2.
in source:	[WRA93] IRS 2
Ref:	=2012ApJ...746...71C
by	CARRASCO-GONZALEZ C. , OSORIO M., ANGLADA G., D'ALESSIO P., RODRIGUEZ L.F., GOMEZ J.F., TORRELLES J.M.
	Astrophys. J., 746, 71 (2012)
	Multiplicity, disks, and jets in the NGC 2071 star-forming region.
o	Fig. 1, Table 2: <[COA2012] IRS 2A> (Nos IRS 2A-IRS 2B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [COB2018]
[COB2018]	(Corti+Orellana+Bosch, 2018)
Write:	<<[COB2018] NNNN>>
N:	248
Object:	Poss. OB* (SIMBAD class: Star)
Note:	CTIO 1-m Curtis Schmidt telescope UBV observations of N=248 candidate members of the OB association Bochum 7. Use of 2MASS and IRAS data.
in source:	Cl Bochum 7
Ref:	=2018A&A...616A..40C
by	CORTI M.A. , ORELLANA R.B., BOSCH G.L.
	Astron. Astrophys., 616A, 40-40 (2018)
	A search for OB stars in the field of the galactic OB association Bochum 7. II. Proper motion and IR photometry.
o	Tables 1-3: <[COB2018] NNNN> N=248 among (Nos 7-4903). Table 2: <[CBN2007] JHHMMSS.s+DDMMSS> N=10 added.
=E=	Catalogue in electronic form as <J/A+A/616/A40/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [COC99]
[COC99]	(Cote+Oke+Cohen, 1999)
Write:	<<[COC99] NN>>
N:	50
Object:	Red Giant (SIMBAD class: Star)
Note:	Keck II LRIS observations
in source:	And II
Ref:	=1999AJ....118.1645C
by	COTE P. , OKE J.B., COHEN J.G.
	Astron. J., 118, 1645-1656 (1999)
	Abundances of red giants in the Andromeda II dwarf spheroidal galaxy.
o	p.1648: stars ANNN = [OA85] NNN
o	Table 1: <[COC99] NN> (Nos 1-50).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: COCD
COCD	(Catalogue of Open Cluster Data)
*****	Avoid the usage of COCD, prefer [KPR2004b]
Origin	of the Acronym: L (2006A&A...445..545P)
Details on Acronym: COCD
COCD	(Catalogue of Open Cluster Data)
*****	Avoid the usage of COCD, prefer [KPR2005]
Origin	of the Acronym: L (2006A&A...445..545P)
Details on Acronym: CoD
CoD	(Cordoba obs., Durchmusterung)
====>	Equivalent to: CD
Details on Acronym: CoD-29 8887X
CoD-29 8887X	(CoD-29 8887, X-ray)
*****	Avoid the usage of CoD-29 8887X, prefer [HHP98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [COG2014]
[COG2014]	(Chiang+Overzier+Gebhardt, 2014)
Write:	<<[COG2014] NN>> <<[COG2014] PCNN>> (not recognised by Simbad, but found in literature)
N:	36
Object:	Poss. Protocluster (SIMBAD class: ClG_Candidate = Cluster of Galaxies Candidate)
Note:	N=36 protocluster candidates in the COSMOS/UltraVISTA field.
in source:	NAME COSMOS Field
Ref:	=2014ApJ...782L...3C
by	CHIANG Y.-K. , OVERZIER R., GEBHARDT K.
	Astrophys. J., 782L, 3 (2014)
	Discovery of a large number of candidate protoclusters traced by ~15 mpc-scale galaxy overdensities in COSMOS.
o	Table 1: <[COG2014] NN> (Nos 1-36).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [COH94]
[COH94]	(Carilli+Owen+Harris, 1994)
Write:	<<[COH94] 0902+343 AN>>
N:	7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio components of the radio galaxy B2 0902+34 Map in Fig.2
in source:	B2 0902+34
Ref:	=1994AJ....107..480C
by	CARILLI C.L. , OWEN F.N., HARRIS D.E.
	Astron. J., 107, 480-493 (1994)
	Radio continuum polarimetric imaging of high redshift radio galaxies.
o	(Erratum) erratum AJ 107 p. 2299
o	Table 2: <Ch90 4C 41.17 A> No. N added. Table 3: <[COH94] 0902+343 AN> (Nos A1-A2, B1-B2, J1-J2, N>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Cohen
Cohen	(Cohen)
*****	Avoid the usage of Cohen, prefer RNO
Details on Acronym: CoKu
CoKu	(Cohen+Kuhi)= (CK)
Write:	<<CoKu {UZ Tau} {f\|p}>> <<CoKu DO Tau East>> <<CoKu {LkHA 346} W{f\|p}>> <<CoKu AA CCC GN>> <<CoKu LkHA NNN GN>> <<CoKu Haro 2-249 GN>> <<CoKu Ser GN>> <<CoKu NGC NNNN Star N>> <<CoKu Tau-Aur Star N>> <<CoKu Mon R2 Star N>> <<CoKu Small Group Star N>> <<CoKu NGC 7000/IC 5070 IRS N>> <<CoKu AA CCC c>> <<CoKu V447 Ori c>> <<CoKu Haro N-NNN c>> <<CoKu LkHA NNN c>> <<CoKu AS NNN c>> <<CoKu Parenago NNNN c>> <<CoKu Ser G1 c>> <<CoKu SR 24 c>> <<CoKu MWC 1080 c>>
N:	90
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	In the format the letter 'G' stands for 'small Group of stars', around another star. At the end of the format the letter 'a' stands for 'f' (forwarding) or 'p' (precessing) At the end of the format the letter 'c' stands for 'companion' of another star. The formats are often found ending with '/GN', '/N', '/IRSN', or '/c'.
Ref:	=1979ApJS...41..743C
by	COHEN M. , KUHI L.V.
	Astrophys. J., Suppl. Ser., 41, 743-843 (1979)
	Observational studies of pre-main-sequence evolution.
o	<CoKu UZ Tau a>, <CoKu DO Tau East>, <CoKu LkHA 346 Na>, <CoKu AA CCC GN>, <CoKu LkHA NNN GN>, <CoKu Haro 2-249 GN>, <CoKu Ser GN> N=39. <CoKu NGC NNNN Star N>, <CoKu Tau-Aur Star N>, <CoKu Mon R2 Star N>, <CoKu Small Group N>, <CoKu NGC 7000/IC 5070 IRS N>, <CoKu AA CCC c>, <CoKu V447 Ori c>, <CoKu Haro N-NNN c>, <CoKu LkHA NNN c> <CoKu AS NNN c>, <CoKu Parenago NNNN c>, <CoKu Ser G1 c>, <CoKu MWC 1080 c> N=81
Origin	of the Acronym: L = Found in the literature
Details on Acronym: COLDz
COLDz	(CO Luminosity Density at High Redshift survey)
Write:	<<COLDz JHHMMSS.ss+DDMMSS.s>> <<COLDz .COS.NN>> <<COLDz .GN.NN>> <<COLDz .GN.R1>> <<COLDz .GN.S1>> <<COLDz -cont-COS-N>> <<COLDz -cont-GN-NN>>
N:	1+26+32+1+1+5+13
Object:	G + Poss. Em. G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLA CO(1-0) and CO(2-1) emission line observations of N=1 star-forming galaxy and N=26 emission-line galaxy candidates in the COSMOS field, and N=32 emission-line galaxy candidates in the GOODS North field. N=2 additional galaxies in the GOODS North field. VLA 34GHz continuum observations of N=5+13 galaxies in the COSMOS and GOODS North field respectively. Use of HST ACS data. For more information, visit: http://coldz.astro.cornell.edu/
in source:	NAME COSMOS Field
in source:	NAME GOODS North Field
Ref:	=2015ApJ...800...67L
by	LENTATI L. , WAGG J., CARILLI C.L., RIECHERS D., CAPAK P., WALTER F., ARAVENA M., DA CUNHA E., HODGE J.A., IVISON R.J., SMAIL I., SHARON C., DADDI E., DECARLI R., DICKINSON M., SARGENT M., SCOVILLE N., SMOLCC V.
	Astrophys. J., 800, 67 (2015)
	COLDz: Karl G. Jansky very large array discovery of a gas-rich galaxy in COSMOS.
o	Fig.1-2, text: <COLDz JHHMMSS.ss+DDMMSS.s> N=1.
Ref:	=2018ApJ...864...49P
by	PAVESI R. , SHARON C.E., RIECHERS D.A., HODGE J.A., DECARLI R., WALTER F., CARILLI C.L., DADDI E., SMAIL I., DICKINSON M., IVISON R.J., SARGENT M., DA CUNHA E., ARAVENA M., DARLING J., SMOLCIC V., SCOVILLE N.Z., CAPAK P.L., WAGG J.
	Astrophys. J., 864, 49-49 (2018)
	The CO Luminosity Density at High-z (COLDz) survey: a sensitive, large-area blind search for low-J CO emission from cold gas in the early universe with the Karl G. Jansky Very Large Array.
o	Tables 3+7: <COLDz .COS.NN> (Nos 0-25), <COLDz .GN.NN> (Nos 0-31). Fig. 7: <COLDz .GN.R1> N=1, <COLDz .GN.S1> N=1.
Ref:	=2021ApJ...912...73A
by	ALGERA H.S.B. , HODGE J.A., RIECHERS D., MURPHY E.J., PAVESI R., ARAVENA M., DADDI E., DECARLI R., DICKINSON M., SARGENT M., SHARON C.E., WAGG J.
	Astrophys. J., 912, 73-73 (2021)
	COLDz: deep 34 GHz continuum observations and free-free emission in high-redshift star-forming galaxies.
o	Fig. 6, Table 1: <COLDz -cont-COS-N> (Nos 1-5), <COLDz -cont-GN-NN> (Nos 1-13).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Collinder
Collinder	(Collinder)= (Cr) = (Lk) = (Lundmark)
Write:	<<Cl Collinder NNN>>
N:	471
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Ref:	=1931AnLun...2....1C
by	COLLINDER P.
	Ann. Obs. Lund, 2, 1-None (1931)
	On structured properties of open galactic clusters and their spatial distribution.
o	<Cl Collinder NNN> (Nos 1-471).
Details on Acronym: com
com	(Comment)
Write:	<<com AAAAAAAAAAAAAAAAAA>>
Object:	Unknown (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	In SIMBAD only, no more in use in SIMBAD 4. The prefix 'com' in SIMBAD is used to indicate a comment. such 'identifiers' should never be taken as designations !
Details on Acronym: [COM2016]
[COM2016]	(Crighton+O'Meara+Murphy, 2016) (Not yet in Simbad)
Write:	<<[COM2016] LLS1249>>
N:	1
Object:	LLS (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=1 Lyman limit system (LLS) at z=3.53 towards the background quasar SDSS J124957.23-015928.8. Use of VLT UVES archival data.
Ref:	=2016MNRAS.457L..44C
by	CRIGHTON N.H.M. , O'MEARA J.M., MURPHY M.T.
	Mon. Not. R. Astron. Soc., 457L, 44-48 (2016)
	Possible Population III remnants at redshift 3.5.
o	<[COM2016] LLS1249> N=1.
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: Coma
Coma	(Coma)
*****	Avoid the usage of Coma, prefer [D80]
Origin	of the Acronym: L (1996ApJS..106....1W)
Details on Acronym: Coma
Coma	(Hammer+Verdoes Kleijn+Hoyos+, 2010)
*****	Avoid the usage of Coma, prefer [HVH2010]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Coma
Coma	(Coma)
*****	Avoid the usage of Coma, prefer [O76b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Coma
Coma	(Coma)
*****	Avoid the usage of Coma, prefer [SS78]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CoMaC
CoMaC	(Coyne+MacConnell)
Write:	<<CoMaC N>>
N:	3
Object:	Poss. PN (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
Stat:	is completely incorporated in Simbad
Note:	CoMaC 1 = VES 866, CoMaC 3 = VES 905 are poss. PN, CoMaC 2 is rejected as a PN in 1992, Acker+ catalog.
Ref:	=1983VatOP...2...73C
by	COYNE G.V. , MacCONNELL D.J.
	Vatican Obs. Publ., 2, 73-None (1983)
	A survey for H-α emission objects in the Milky Way. VII. Final zones.
o	(g1F) coord fournies par Brian (FW 14/5/09). CoMaC 1 = Em* VES 866, CoMaC 2 = Em* VES 905
o	<EM* VES NNN> (Nos 681-977). <CoMaC N> (Nos 1-3)
=E=	Catalogue in electronic form as III/256
Origin	of the Acronym: L (1992ESOPN...1....1A)
Details on Acronym: ComaCC
ComaCC	(Coma Cluster Catalogue)= CCC
Write:	<<ComaCC NNN>>
N:	774
Object:	G (SIMBAD class: Galaxy)
Note:	The Coma Cluster Catalogue (N=774 galaxies) is part of a far-infrared survey of the Coma cluster and the galaxy filament it resides within. See also the Coma Filament Catalogue (ComaFC). Use of H-ATLAS and SDSS data.
in source:	ACO 1656 = Coma Cluster
Ref:	=2016MNRAS.458..582F
by	FULLER C. , DAVIES J.I., SMITH M.W.L., VALIANTE E., EALES S., BOURNE N., DUNNE L., DYE S., FURLANETTO C., IBAR E., IVISON R., MADDOX S., SANSOM A., MICHALOWSKI M.J., DAVIS T.
	Mon. Not. R. Astron. Soc., 458, 582-602 (2016)
	H-ATLAS: the far-infrared properties of galaxies in and around the Coma cluster.
o	Table A.1: <ComaCCNNN> (Nos 001-774). Table B.1: <ComaFCNNN> (Nos 001-951).
=E=	Catalogue in electronic form as <J/MNRAS/458/582/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ComaFC
ComaFC	(Coma Filament Catalogue)= CFC
Write:	<<ComaFC NNN>>
N:	951
Object:	G (SIMBAD class: Galaxy)
Note:	The Coma Filament Catalogue (N=951 galaxies) is part of a far-infrared survey of the Coma cluster and the galaxy filament it resides within. See also the Coma Cluster Catalogue (ComaCC). Use of H-ATLAS and SDSS data.
in source:	ACO 1656 = Coma Cluster
Ref:	=2016MNRAS.458..582F
by	FULLER C. , DAVIES J.I., SMITH M.W.L., VALIANTE E., EALES S., BOURNE N., DUNNE L., DYE S., FURLANETTO C., IBAR E., IVISON R., MADDOX S., SANSOM A., MICHALOWSKI M.J., DAVIS T.
	Mon. Not. R. Astron. Soc., 458, 582-602 (2016)
	H-ATLAS: the far-infrared properties of galaxies in and around the Coma cluster.
o	Table A.1: <ComaCCNNN> (Nos 001-774). Table B.1: <ComaFCNNN> (Nos 001-951).
=E=	Catalogue in electronic form as <J/MNRAS/458/582/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: COMBO
COMBO	(Classification of Objects by Medium-Band Observation)
Write:	<<COMBO JHHMMSSs+DDMMSS>>
N:	63501
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	MPG/ESO 2.2m telescope multi-band photometry of three fields including the Chandra Deep Field South (CDFS). See also [WDK2001].
in source:	NAME CDFS
in source:	NAME ACO 901-902 Supercluster
Ref:	=2001A&A...377..442W
by	WOLF C. , DYE S., KLEINHEINRICH M., MEISENHEIMER K., RIX H.-W., WISOTZKI L.
	Astron. Astrophys., 377, 442-449 (2001)
	Deep BVR photometry of the Chandra Deep Field South from the COMBO-17 survey.
o	Table 3: <[WDK2001] NNNNN> (Nos 1-63501) = <COMBO JHHMMSSs+DDMMSS> N=63501.
Ref:	=2009MNRAS.393.1275G
by	GRAY M.E. , WOLF C., BARDEN M., PENG C.Y., HAUSSLER B., BELL E.F., McINTOSH D.H., GUO Y., CALDWELL J.A.R., BACON D., BALOGH M., BARAZZA F.D., BOHM A., HEYMANS C., JAHNKE K., JOGEE S., VAN KAMPEN E., LANE K., MEISENHEIMER K., SANCHEZ S.F., TAYLOR A., WISOTZKI L., ZHENG X., GREEN D.A., BESWICK R.J., SAIKIA D.J., GILMOUR R., JOHNSON B.D., PAPOVICH C.
	Mon. Not. R. Astron. Soc., 393, 1275-1301 (2009)
	STAGES: the Space Telescope A901/2 Galaxy Evolution Survey.
o	<STAGES FF-NNNN> N=75805. <COMBO JHHMMSSs+DDMMSS> = <[GWB2009] NNNNN> N=63775.
=E=	Catalogue in electronic form as J/A+A/377/442
=E=	Catalogue in electronic form as II/253
=E=	Catalogue in electronic form as J/MNRAS/393/1275
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: COMBO-17
COMBO-17	(COMBO-17)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Complex
Complex	(Complex)
*****	Avoid the usage of Complex, prefer [H68]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CoO
CoO	(Cordoba Obs.)
Write:	<<** COO NNNAA>>
Object:	(SIMBAD class: = Double or Multiple Star)
Note:	Supersedes Cor, IDS Nomenclature.
Rem:	Obsolete
Details on Acronym: COOL
COOL	(ChicagO Optically-selected Lenses)
Write:	<<COOL JHHMM+HHMM system>> <<COOL JHHMM+HHMM lens>> <<COOL JHHMM+HHMM source>>
Object:	Grav. lens system + Grav. lens + G + QSO (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Lensed galaxies in strong-lensing systems, as part of the COOL-LAMPS (ChicagO Optically-selected Lenses - Located At the Margins of Public Surveys) project. More information available on the collaboration website: https://coollamps.github.io
Ref:	=2021ApJ...906..107K
by	KHULLAR G. , GOZMAN K., LIN J.J., MARTINEZ M.N., ACUNA O.S.M., MEDINA E., MERZ K., SANCHEZ J.A., SISCO E.E., KAVIN STEIN D.J., SUKAY E.O., TAVANGAR K., BAYLISS M.B., BLEEM L.E., BROWNSBERGER S., DAHLE H., FLORIAN M.K., GLADDERS M.D., MAHLER G., RIGBY J.R., SHARON K., STARK A.A.
	Astrophys. J., 906, 107-107 (2021)
	COOL-LAMPS. I. An extraordinarily bright lensed galaxy at redshift 5.04.
o	<COOL J1241+2219 system> N=1. <COOL J1241+2219 lens> N=1. <COOL J1241+2219 source> N=1. <[KGL2021] COOL J1241+2219 arc> N=1.
Ref:	=2022ApJ...940...42S
by	SUKAY E. , KHULLAR G., GLADDERS M.D., SHARON K., MAHLER G., NAPIER K., BLEEM L.E., DAHLE H., FLORIAN M.K., GOZMAN K., LIN J.J., MARTINEZ M.N., MATTHEWS ACUNA O.S., MEDINA E., MERZ K., SANCHEZ J.A., SISCO E.E., KAVIN STEIN D.J., TAVANGAR K., WHITAKER K.E.
	Astrophys. J., 940, 42 (2022)
	COOL-LAMPS. II. Characterizing the Size and Star Formation History of a Bright Strongly Lensed Early-type Galaxy at Redshift 1.02.
o	<COOL J1323+0343 system> N=1. <COOL J1323+0343 lens> N=1. <COOL J1323+0343 source> N=1. <[SKG2022] COOL J1323+0343 N> (Nos 1-4). <[SKG2022] COOL J1323+0343 arc> N=1.
Ref:	=2023ApJ...946...63M
by	MARTINEZ M.N. , NAPIER K.A., CLOONAN A.P., SUKAY E., GOZMAN K., MERZ K., KHULLAR G., LIN J.J., MATTHEWS ACUNA O.S., MEDINA E., SANCHEZ J.A., SISCO E.E., KAVIN STEIN D.J., TAVANGAR K., GONZALEZ J.R., MAHLER G., SHARON K., DAHLE H., GLADDERS M.D.
	Astrophys. J., 946, 63 (2023)
	COOL-LAMPS. III. Discovery of a 25.''9 Separation Quasar Lensed by a Merging Galaxy Cluster.
o	<COOL J0542-2125 system> N=1. <COOL J0542-2125 lens> N=1. <COOL J0542-2125 source> N=1. Figs 1+3, Table 1: <[MNC2023] COOL J0542-2125 AN> (Nos A-C, A1-A3, B1-B2, C1-C3). Fig. 5, Table 2: <[MNC2023] COOL J0542-2125 N.N> (Nos 1.1-1.3 to 5.1-5.2).
Ref:	=2023ApJ...950...58Z
by	ZHANG Y. , MANWADKAR V., GLADDERS M.D., KHULLAR G., DAHLE H., NAPIER K.A., MAHLER G., SHARON K., MATTHEWS ACUNA O.S., ASHMEAD F., CERNY W., GONZALEZ J.R., GOZMAN K., LEVINE B.C., MAROHNIC D., MARTINEZ M.N., MERZ K., PAN Y., SANCHEZ J.A., SIERRA I., SISCO E.E., SUKAY E., TAVANGAR K., ZABOROWSKI E.
	Astrophys. J., 950, 58 (2023)
	COOL-LAMPS. IV. A Sample of Bright Strongly Lensed Galaxies at 3 < z < 4.
o	Tables 1-2: <COOL JHHMM+DDMM system> N=5, <COOL JHHMM+DDMM lens> N=5, <COOL JHHMM+DDMM source> N=5. Fig. 8: <[ZMG2023] JHHMM+DDMM N.N> N=6+14+9+10+9, <[ZMG2023] J0104-0757 GN> (Nos G1-G2).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: COP
COP	(Canada-France-Hawaii Optical PDCS survey)
Write:	<<COP PDCS NN NN.NN>> <<COP PDCS NN-NN NN.NN>>
N:	635
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=635 galaxies in 11 PDCS ClG.
in source:	PDCS 4
in source:	PDCS 16
in source:	PDCS 30
in source:	PDCS 45
in source:	PDCS 33
in source:	PDCS 34
in source:	PDCS 38
in source:	PDCS 57
in source:	PDCS 61
in source:	PDCS 62
in source:	PDCS 67
Ref:	=2000AJ....120....1A
by	ADAMI C. , HOLDEN B.P., CASTANDER F.J., NICHOL R.C., MAZURE A., ULMER M.P., POSTMAN M., LUBIN L.M.
	Astron. J., 120, 1-22 (2000)
	The Canada-France-Hawaii telescope optical PDCS survey (COP). I. The data.
o	Tables 6-15: <COP PDCS NN NN.NN>, <COP PDCS 30-45 NN.NN>, N=74+53+88+71+51+152+22+83+41.
=E=	Catalogue in electronic form as J/AJ/120/1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [COP2011]
[COP2011]	(Chauhan+Ogura+Pandey+, 2011)
Write:	<<[COP2011] NNa>>
N:	15
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Himalayan Chandra 2m telescope (HCT, India) HFOSC VI photometric observations of stars in the southeastern part of IC 1848E.
in source:	IC 1848A
Ref:	=2011PASJ...63..795C
by	CHAUHAN N. , OGURA K., PANDEY A.K., SAMAL M.R., BHATT B.C.
	PASJ, 63, 795-802 (2011)
	Stars at the tip of peculiar elephant trunk-like clouds in IC 1848E: A possible third mechanism of triggered star formation.
o	Tables 1, 3-4: <[COP2011] NNa> (Nos 1a-1b, 2-12, 13a-13b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Cor
Cor	(Cordoba obs.)
Write:	<<** COR NNN>>
Object:	(SIMBAD class: = Double or Multiple Star)
Rem:	Obsolete. IDS Nomenclature.
Details on Acronym: Cornell
Cornell	(Cornell univ.) (Not yet in Simbad)
Write:	<<Cornell N>>
N:	2
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Details on Acronym: CORNISH
CORNISH	(Co-Ordinated Radio 'N' Infrared Survey for High-mass star formation)
Write:	<<CORNISH GLLL.llll+BB.bbbb>>
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	The CORNISH project ("Co-Ordinated Radio 'N' Infrared Survey for High-mass star formation") is the radio continuum part of a series of multi-wavelength surveys of the Galactic Plane that focus on the northern GLIMPSE region (l=10° to 65°, \|b\|<1°), completed by the Spitzer space telescope in the mid-IR. CORNISH uses the VLA in B and BnA configurations at 5GHz. The CORNISH data and catalog are available online at http://cornish.leeds.ac.uk
Ref:	=2013ApJS..205....1P
by	PURCELL C.R. , HOARE M.G., COTTON W.D., LUMSDEN S.L., URQUHART J.S., CHANDLER C., CHURCHWELL E.B., DIAMOND P., DOUGHERTY S.M., FENDER R.P., FULLER G., GARRINGTON S.T., GLEDHILL T.M., GOLDSMITH P.F., HINDSON L., JACKSON J.M., KURTZ S.E., MARTI J., MOORE T.J.T., MUNDY L.G., MUXLOW T.W.B., OUDMAIJER R.D., PANDIAN J.D., PAREDES J.M., SHEPHERD D.S., SMETHURST S., SPENCER R.E., THOMPSON M.A., UMANA G., ZIJLSTRA A.A.
	Astrophys. J., Suppl. Ser., 205, 1 (2013)
	The CoOrdinated Radio and Infrared Survey for High-mass star formation. II. Source catalog.
o	Table 3: <CORNISH GLLL.llll+BB.bbbb> N=2637.
=E=	Catalogue in electronic form as J/ApJS/205/1
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CoRoT
CoRoT	(Convection, Rotation, Transit)= (CoRoT-Exo)
Write:	<<CoRoT NNNNNNNNN>> <<CoRoT -NN>> <<CoRoT -NNa>>
Object:	* + Poss. Planet (SIMBAD class: Star)
Note:	COROT search for exoplanets. Format NNNNNNNNN: COROT target stars (numbers larger than 100000000 are for stars observed in the faint star mode, numbers smaller than 22000 for stars observed in the bright star mode). Format -NN: stars with extra-solar planet candidates. Format -NNa: extra-solar planet candidates. Only the first references using these formats are given here.
Ref:	=2007ApJ...667L.191L
by	LOPEZ-MORALES M. , SEAGER S.
	Astrophys. J., 667L, 191-194 (2007)
	Thermal emission from transiting very hot Jupiters: prospects for ground-based detection at optical wavelengths.
o	Table 1: <CoRoT-N> (No. 1), <CoRoT-Na> (No. 1b).
Ref:	=2008A&A...479..865L
by	LOEILLET B. , BOUCHY F., DELEUIL M., ROYER F., BOURET J.-C., MOUTOU C., BARGE P., DE LAVERNY P., PONT F., RECIO-BLANCO A., SANTOS N.C.
	Astron. Astrophys., 479, 865-875 (2008)
	Doppler search for exoplanet candidates and binary stars in a CoRoT field using a multi-fiber spectrograph. I. Global analysis and first results.
o	Tables 3, 4, 5: <CoRoT NNNNNNNNN> N=50+9+14.
Ref:	=2008A&A...482L..21A
by	ALONSO R. , AUVERGNE M., BAGLIN A., OLLIVIER M., MOUTOU C., ROUAN D., DEEG H.J., AIGRAIN S., ALMENARA J.-M., BARBIERI M., BARGE P., BENZ W., BORDE P., BOUCHY F., DE LA REZA R., DELEUIL M., DVORAK R., ERIKSON A., FRIDLUND M., GILLON M., GONDOIN P., GUILLOT T., HATZES A., HEBRARD G., KABATH P., JORDA L., LAMMER H., LEGER A., LLEBARIA A., LOEILLET B., MAGAIN P., MAYOR M., MAZEH T., PAETZOLD M., PEPE F., PONT F., QUELOZ D., RAUER H., SHPORER A., SCHNEIDER J., STECKLUM B., UDRY S., WUCHTERL G.
	Astron. Astrophys., 482L, 21-24 (2008)
	Transiting exoplanets from the CoRoT space mission. II. CoRoT-Exo-2b: a transiting planet around an active G star.
o	<CoRoT-N> (No. 2), <CoRoT-Na> (No. 2b).
Ref:	=2008A&A...488L..43A
by	AIGRAIN S. , COLLIER CAMERON A., OLLIVIER M., PONT F., JORDA L., ALMENARA J.M., ALONSO R., BARGE P., BORDE P., BOUCHY F., DEEG H., DE LA REZA R., DELEUIL M., DVORAK R., ERIKSON A., FRIDLUND M., GONDOIN P., GILLON M., GUILLOT T., HATZES A., LAMMER H., LANZA A.F., LEGER A., LLEBARIA A., MAGAIN P., MAZEH T., MOUTOU C., PAETZOLD M., PINTE C., QUELOZ D., RAUER H., ROUAN D., SCHNEIDER J., WUCHTER G., ZUCKER S.
	Astron. Astrophys., 488L, 43-46 (2008)
	Transiting exoplanets from the CoRoT space mission. IV. CoRoT-Exo-4b: a transiting planet in a 9.2 day synchronous orbit.
o	<CoRoT-N> (No. 4). <CoRoT-Na> (No. 4b).
Ref:	=2008A&A...491..889D
by	DELEUIL M. , DEEG H.J., ALONSO R., BOUCHY F., ROUAN D., AUVERGNE M., BAGLIN A., AIGRAIN S., ALMENARA J.M., BARBIERI M., BARGE P., BRUNTT H., BORDE P., COLLIER CAMERON A., CSIZMADIA Sz., DE LA REZA R., DVORAK R., ERIKSON A., FRIDLUND M., GANDOLFI D., GILLON M., GUENTHER E., GUILLOT T., HATZES A., HEBRARD G., JORDA L., LAMMER H., LEGER A., LLEBARIA A., LOEILLET B., MAYOR M., MAZEH T., MOUTOU C., OLLIVIER M., PAETZOLD M., PONT F., QUELOZ D., RAUER H., SCHNEIDER J., SHPORER A., WUCHTERL G., ZUCKER S.
	Astron. Astrophys., 491, 889-897 (2008)
	Transiting exoplanets from the CoRoT space mission . VI. CoRoT-Exo-3b: the first secure inhabitant of the brown-dwarf desert.
o	<CoRoT-N> (No. 3), <CoRoT-Na> (No. 3b).
=E=	Catalogue in electronic form as B/corot/Faint_star
=E=	Catalogue in electronic form as B/corot/Bright_star
=E=	Catalogue in electronic form as J/A+A/479/865
=E=	Catalogue in electronic form as <J/A+A/491/889/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CoRoT-Exo
CoRoT-Exo	(Convection, Rotation, Transit, exoplanet)
*****	Avoid the usage of CoRoT-Exo, prefer CoRoT
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: COS
COS	(Cudworth+Olszewski+Schommer)= [COS86] = (Cud) = (EDO)
Write:	<<COS NNN>>
N:	530
Object:	* (SIMBAD class: Star)
Note:	Table V
in source:	NAME UMi Dwarf Galaxy
Ref:	=1986AJ.....92..766C
by	CUDWORTH K.M. , OLSZEWSKI E.W., SCHOMMER R.A.
	Astron. J., 92, 766-776 (1986)
	Proper motions and bright-star photometry in the Ursa Minor dwarf galaxy.
o	Table V: <COS NNN> (Nos 1-530)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CoS
CoS	(Coalsack DCld)
*****	Avoid the usage of CoS, prefer [VMF94]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [COS86]
[COS86]	(Cudworth+Olszewski+Schommer, 1986)
====>	Equivalent to: COS
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: COSBO
COSBO	(Cosmic Evolution Survey, MAMBO)
*****	Avoid the usage of COSBO, prefer COSMOSMAMBO
Origin	of the Acronym: L (2012A&A...548A...4S)
Details on Acronym: COSLA
COSLA	(Cosmic Evolution Survey, LABOCA)
*****	Avoid the usage of COSLA, prefer COSMOSLABOCA
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: COSMOS
COSMOS	(Cosmic Evolution Survey with HST)
Write:	<<COSMOS JHHMMSS.ss+DDMMSS.s>> <<COSMOS NNNNNNN>>
N:	about 2000000
Object:	G (SIMBAD class: Galaxy)
Note:	The Cosmic Evolution Survey is an HST Treasury Project to survey a 2 square degree equatorial field with ACS. The field is centered on: 10:00:28.6 +02:12:21.0 so all of the objects with the COSMOS acronym should be within about a degree of that position. The COSMOS web site is: http://cosmos.astro.caltech.edu/ The survey is described in 2007ApJS..172....1S. 2006MNRAS.370..477L: ref. with 7 COSMOS galaxies (format JHHMMSS.ss+DDMMSS.s). 2007ApJS..172...99C : first release (format NNNNNNN).
Ref:	=2006MNRAS.370..477L
by	LISKER T. , DEBATTISTA V.P., FERRERAS I., ERWIN P.
	Mon. Not. R. Astron. Soc., 370, 477-487 (2006)
	Double-barred galaxies at intermediate redshifts: a feasibility study.
o	Fig.3, Table 1: <[LDF2006] S2B N> (Nos 1-2). Table 2: <COSMOS JHHMMSS.ss+DDMMSS.s> N=7.
Ref:	=2007ApJS..172...99C
by	CAPAK P. , AUSSEL H., AJIKI M., McCRACKEN H.J., MOBASHER B., SCOVILLE N., SHOPBELL P., TANIGUCHI Y., THOMPSON D., TRIBIANO S., SASAKI S., BLAIN A.W., BRUSA M., CARILLI C., COMASTRI A., CAROLLO C.M., CASSATA P., COLBERT J., ELLIS R.S., ELVIS M., GIAVALISCO M., GREEN W., GUZZO L., HASINGER G., ILBERT O., IMPEY C., JAHNKE K., KARTALTEPE J., KNEIB J.-P., KODA J., KOEKEMOER A., KOMIYAMA Y., LEAUTHAUD A., LEFEVRE O., LILLY S., LIU C., MASSEY R., MIYAZAKI S., MURAYAMA T., NAGAO T., PEACOCK J.A., PICKLES A., PORCIANI C., RENZINI A., RHODES J., RICH M., SALVATO M., SANDERS D.B., SCARLATA C., SCHIMINOVICH D., SCHINNERER E., SCODEGGIO M., SHETH K., SHIOYA Y., TASCA L.A.M., TAYLOR J.E., YAN L., ZAMORANI G.
	Astrophys. J., Suppl. Ser., 172, 99-116 (2007)
	The first release COSMOS optical and Near-IR data and catalog.
o	<COSMOS NNNNNNN> N=438226.
=E=	Catalogue in electronic form as II/284
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: COSMOS
COSMOS	(Cosmic Evolution Survey with HST)
*****	Avoid the usage of COSMOS, prefer [FKC2008]
Details on Acronym: COSMOS
COSMOS	(Cosmic Evolution Survey)
*****	Avoid the usage of COSMOS, prefer [ICS2009]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: COSMOS
COSMOS	(Cosmic Evolution Survey with HST)
*****	Avoid the usage of COSMOS, prefer [TIM2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: COSMOS-XS
COSMOS-XS	(COSMOS - X-band and S-band)= (CXS)
Write:	<<COSMOS-XS JHHMMSS.ss+DDMMSS.ss>>
N:	91+1498
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Karl G. Jansky Very Large Array observations at 10GHz (X-band) and 3GHz (S-band) of N=91+1498 sources in the COSMOS field.
in source:	NAME COSMOS Field
Ref:	=2021ApJ...907....5V
by	VAN DER VLUGT D. , ALGERA H.S.B., HODGE J.A., NOVAK M., RADCLIFFE J.F., RIECHERS D.A., ROTTGERING H., SMOLCIC V., WALTER F.
	Astrophys. J., 907, 5-5 (2021)
	An ultradeep multiband VLA survey of the faint radio sky (COSMOS-XS): source catalog and number counts.
o	<COSMOS-XS JHHMMSS.ss+DDMMSS.ss> N=91+1498.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: COSMOS2015
COSMOS2015	(COSMOS2015)
Write:	<<COSMOS2015 NNNNNNN>>
N:	1182108
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	COSMOS2015 catalog in the COSMOS field. Use of UltraVISTA-DR2, Subaru HSC, Spitzer data.
in source:	NAME COSMOS Field
Ref:	=2016ApJS..224...24L
by	LAIGLE C. , McCRACKEN H.J., ILBERT O., HSIEH B.C., DAVIDZON I., CAPAK P., HASINGER G., SILVERMAN J.D., PICHON C., COUPON J., AUSSEL H., LE BORGNE D., CAPUTI K., CASSATA P., CHANG Y.-Y., CIVANO F., DUNLOP J., FYNBO J., KARTALTEPE J.S., KOEKEMOER A., LE FEVRE O., LE FLOC'H E., LEAUTHAUD A., LILLY S., LIN L., MARCHESI S., MILVANG-JENSEN B., SALVATO M., SANDERS D.B., SCOVILLE N., SMOLCIC V., STOCKMANN M., TANIGUCHI Y., TASCA L., TOFT S., VACCARI M., ZABL J.
	Astrophys. J., Suppl. Ser., 224, 24-24 (2016)
	The COSMOS2015 catalog: exploring the 1 < z < 6 universe with half a million galaxies.
o	Catalog: <COSMOS2015 NNNNNNN> (Nos 1-1182108).
=E=	Catalogue in electronic form as <J/ApJS/224/24/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: COSMOS2020
COSMOS2020	(COSMOS2020)
Write:	<<COSMOS2020 Classic NNNNNNN>> <<COSMOS2020 Farmer NNNNNNN>>
N:	1720700+964506
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Source detection and multiwavelength photometry for N=1720700+964506 sources in the COSMOS field in two independent catalogs, the "Classic" and the "Farmer" respectively. Use of UltraVISTA-DR4.1 data. See also COSMOS2015.
in source:	NAME COSMOS Field
Ref:	=2022ApJS..258...11W
by	WEAVER J.R. , KAUFFMANN O.B., ILBERT O., McCRACKEN H.J., MONETI A., TOFT S., BRAMMER G., SHUNTOV M., DAVIDZON I., HSIEH B.C., LAIGLE C., ANASTASIOU A., JESPERSEN C.K., VINTHER J., CAPAK P., CASEY C.M., McPARTLAND C.J.R., MILVANG-JENSEN B., MOBASHER B., SANDERS D.B., ZALESKY L., ARNOUTS S., AUSSEL H., DUNLOP J.S., FAISST A., FRANX M., FURTAK L.J., FYNBO J.P.U., GOULD K.M.L., GREVE T.R., GWYN S., KARTALTEPE J.S., KASHINO D., KOEKEMOER A.M., KOKOREV V., LE FEVRE O., LILLY S., MASTERS D., MAGDIS G., MEHTA V., PENG Y., RIECHERS D.A., SALVATO M., SAWICKI M., SCARLATA C., SCOVILLE N., SHIRLEY R., SILVERMAN J.D., SNEPPEN A., SMOLCIC V., STEINHARDT C., STERN D., TANAKA M., TANIGUCHI Y., TEPLITZ H.I., VACCARI M., WANG W.-H., ZAMORANI G.
	Astrophys. J., Suppl. Ser., 258, 11-11 (2022)
	COSMOS2020: a panchromatic view of the Universe to z ~ 10 from two complementary catalogs.
o	<COSMOS2020 Classic NNNNNNN> (Nos 1-1720700). <COSMOS2020 Farmer NNNNNN> (Nos 1-964506).
=E=	Catalogue in electronic form as <J/ApJS/258/11/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: COSMOSLABOCA
COSMOSLABOCA	(Cosmic Evolution Survey, LABOCA)= (COSLA)
Write:	<<COSMOSLABOCA NNNW>>
N:	163
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	APEX Laboca 870µm and IRAM PdBI 1.3mm continuum observations of submillimeter galaxies in the COSMOS field.
in source:	NAME COSMOS Field
Ref:	=2012A&A...548A...4S
by	SMOLCIC V. , ARAVENA M., NAVARRETE F., SCHINNERER E., RIECHERS D.A., BERTOLDI F., FERUGLIO C., FINOGUENOV A., SALVATO M., SARGENT M., McCRACKEN H.J., ALBRECHT M., KARIM A., CAPAK P., CARILLI C.L., CAPPELLUTI N., ELVIS M., ILBERT O., KARTALTEPE J., LILLY S., SANDERS D., SHETH K., SCOVILLE N.Z., TANIGUCHI Y.
	Astron. Astrophys., 548A, 4-4 (2012)
	Millimeter imaging of submillimeter galaxies in the COSMOS field: redshift distribution.
o	Tables 1-6, A.1, B.1: <COSMOSLABOCA NNW> N=49 among (Nos 1-161).
Ref:	=2012A&A...539A.155M
by	MAGNELLI B. , LUTZ D., SANTINI P., SAINTONGE A., BERTA S., ALBRECHT M., ALTIERI B., ANDREANI P., AUSSEL H., BERTOLDI F., BETHERMIN M., BONGIOVANNI A., CAPAK P., CHAPMAN S., CEPA J., CIMATTI A., COORAY A., DADDI E., DANIELSON A.L.R., DANNERBAUER H., DUNLOP J.S., ELBAZ D., FARRAH D., FOERSTER SCHREIBER N.M., GENZEL R., HWANG H.S., IBAR E., IVISON R.J., LE FLOC'H E., MAGDIS G., MAIOLINO R., NORDON R., OLIVER S.J., PEREZ GARCIA A., POGLITSCH A., POPESSO P., POZZI F., RIGUCCINI L., RODIGHIERO G., ROSARIO D., ROSEBOOM I., SALVATO M., SANCHEZ-PORTAL M., SCOTT D., SMAIL I., STURM E., SWINBANK A.M., TACCONI L.J., VALTCHANOV I., WANG L., WUYTS S.
	Astron. Astrophys., 539A, 155-155 (2012)
	A Herschel view of the far-infrared properties of submillimetre galaxies.
o	Tables 9-10: <COSMOSLABOCA NNN> N=6 added among (Nos 2-163).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: COSMOSMAMBO
COSMOSMAMBO	(Cosmic Evolution Survey, MAMBO)= (MAMBO) = (MM) = (COSBO)
Write:	<<COSMOSMAMBO NN>> <<COSMOSMAMBO NNW>> <<COSMOSMAMBO NNWN>> <<COSMOSMAMBO MM JHHMMSS+DDMMSS>>
N:	77+15+2
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	IRAM 30m MAMBO-2 1.2mm observations of the COSMOS field. See also [BCA2007].
in source:	NAME COSMOS Field
Ref:	=2007ApJS..172..132B
by	BERTOLDI F. , CARILLI C., ARAVENA M., SCHINNERER E., VOSS H., SMOLCIC V., JAHNKE K., SCOVILLE N., BLAIN A., MENTEN K.M., LUTZ D., BRUSA M., TANIGUCHI Y., CAPAK P., MOBASHER B., LILLY S., THOMPSON D., AUSSEL H., KREYSA E., HASINGER G., AGUIRRE J., SCHLAERTH J., KOEKEMOER A.
	Astrophys. J., Suppl. Ser., 172, 132-149 (2007)
	COSBO: the MAMBO 1.2 millimeter imaging survey of the COSMOS field.
o	Objects refered as COSMOS 1211238, 1211239, 1240610, 1252837, 1252838, 1259096, 1605942, 1654929, 1654930, 1950977, 1958423, in Table 2 do not exist in the public COSMOS catalogue 2007ApJS..172...99C and have not been created in Simbad.
o	Tables 1,2 col(1): <COSMOSMAMBO NNWN> N=27 among (Nos 1-37) +19 +2. Table 1, col(2): <COSMOSMAMBO MM JHHMMSS+DDMMSS> N=27. Table 1, col(VLA): <[BCA2007] VLA JHHMMSS.ss+DDMMSS.s> N=30.
=E=	Catalogue in electronic form as <II/284/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: COSMOSVLA
COSMOSVLA	(Cosmic Evolution Survey, VLA)
Write:	<<COSMOSVLA JHHMMSS.ss+DDMMSS.s>>
N:	3643
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 1.4GHz observations of the COSMOS field. See alos [SCS2004].
in source:	NAME COSMOS Field
Ref:	=2007ApJS..172...46S
by	SCHINNERER E. , SMOLCIC V., CARILLI C.L., BONDI M., CILIEGI P., JAHNKE K., SCOVILLE N.Z., AUSSEL H., BERTOLDI F., BLAIN A.W., IMPEY C.D., KOEKEMOER A.M., LE FEVRE O., URRY C.M.
	Astrophys. J., Suppl. Ser., 172, 46-69 (2007)
	The VLA-COSMOS survey. II. Source catalog of the large project.
o	Calibrator 0521+166 not identified.
o	Table 3: <COSMOSVLA JHHMMSS.ss+DDMMSS.s> N=3643.
=E=	Catalogue in electronic form as J/ApJS/172/46
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: COSMOSVLA3
COSMOSVLA3	(VLA-COSMOS 3 GHz Large Project)
Write:	<<COSMOSVLA3 JHHMMSS.ss+DDMMSS.s>>
N:	10830
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA-COSMOS 3GHz Large Project catalog of N=10830 radio sources. VLA 3GHz (10cm) observations of the COSMOS field. See also [SNB2017].
in source:	NAME COSMOS Field
Ref:	=2017A&A...602A...1S
by	SMOLCIC V. , NOVAK M., BONDI M., CILIEGI P., MOOLEY K.P., SCHINNERER E., ZAMORANI G., NAVARRETE F., BOURKE S., KARIM A., VARDOULAKI E., LESLIE S., DELHAIZE J., CARILLI C.L., MYERS S.T., BARAN N., DELVECCHIO I., MIETTINEN O., BANFIELD J., BALOKOVIC M., BERTOLDI F., CAPAK P., FRAIL D.A., HALLINAN G., HAO H., HERRERA RUIZ N., HORESH A., ILBERT O., INTEMA H., JELIC V., KLOCKNER H.-R., KRPAN J., KULKARNI S.R., McCRACKEN H., LAIGLE C., MIDDLEBERG E., MURPHY E.J., SARGENT M., SCOVILLE N.Z., SHETH K.
	Astron. Astrophys., 602A, 1-1 (2017)
	The VLA-COSMOS 3 GHz Large Project: Continuum data and source catalog release.
o	Table 5, col(1): <[SNB2017] NNNNN> N=10830 among (Nos 1-10966) = Table 5, col(2): <COSMOSVLA3 JHHMMSS.ss+DDMMSS.s> N=10830.
=E=	Catalogue in electronic form as <J/A+A/602/A1/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: COSMOSVLA327
COSMOSVLA327	(VLA-COSMOS 90cm)
Write:	<<COSMOSVLA327 JHHMMSS.ss+DDMMSS.s>> <<COSMOSVLA327 HHMMSS.ss+DDMMSS.s>> (not recognised by Simbad, but found in literature)
N:	182
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Catalog of N=182 radio sources, extracted from 90cm VLA imaging of the COSMOS field.
in source:	NAME COSMOS Field
Ref:	=2014MNRAS.443.2590S
by	SMOLCIC V. , CILIEGI P., JELIC V., BONDI M., SCHINNERER E., CARILLI C.L., RIECHERS D.A., SALVATO M., BRKOVIC A., CAPAK P., ILBERT O., KARIM A., McCRACKEN H., SCOVILLE N.Z.
	Mon. Not. R. Astron. Soc., 443, 2590-2598 (2014)
	The VLA-COSMOS Survey - V. 324 MHz continuum observations.
o	Table 1: <COSMOSVLA327 JHHMMSS.ss+DDMMSS.s> N=182.
=E=	Catalogue in electronic form as <J/MNRAS/443/2590/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: COSMOSVLADP
COSMOSVLADP	(COSMOS-VLA Deep Project)
Write:	<<COSMOSVLADP JHHMMSS.ss+DDMMSS.s>>
N:	2865
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 1.4GHz observations of the central degree of the COSMOS field.
in source:	NAME COSMOS Field
Ref:	=2010ApJS..188..384S
by	SCHINNERER E. , SARGENT M.T., BONDI M., SMOLCIC V., DATTA A., CARILLI C.L., BERTOLDI F., BLAIN A., CILIEGI P., KOEKEMOER A., SCOVILLE N.Z.
	Astrophys. J., Suppl. Ser., 188, 384-404 (2010)
	The VLA-COSMOS survey. IV. Deep data and joint catalog.
o	Table 3: <COSMOSVLADP JHHMMSS.ss+DDMMSS.s> N=2865.
=E=	Catalogue in electronic form as J/ApJS/188/384
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cou
Cou	(Courtes) (Not yet in Simbad)
*****	Avoid the usage of Cou, prefer [C51]
Details on Acronym: Cou
Cou	(Couteau)= (Couteau)
Write:	<< Cou NNNNAA>> << Cou NNNNAa>>
N:	2700
Object:	(SIMBAD class: = Double or Multiple Star)
Ref:	=1993CED27.C......1C
by	COUTEAU P.
	Obs. Cote d'Azur, Dep. Augustin FRESNEL URA 1361 (2eme Edition), 1-None (1993)
	Catalogue de 2700 etoiles doubles.
o	<** COU NNNN> N=2700
=E=	Catalogue in electronic form as I/209
Details on Acronym: [COU96]
[COU96]	(Chen+Ohashi+Umemoto, 1996)
Write:	<<[COU96] N>>
N:	7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
in source:	Orion Nebula:LDN 1641N = LDN 1641N
Ref:	=1996AJ....112..717C
by	CHEN H. , OHASHI N., UMEMOTO T.
	Astron. J., 112, 717-722 (1996)
	High-resolution millimeter imaging of L 1641N : multiple cores with a young stellar group.
o	Table 1: <[COU96] N> (Nos 1-7)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: COUP
COUP	(Chandra Orion Ultradeep Project)
Write:	<<COUP NNNNa>> <<COUP JHHMMSS.s+DDMMSS>>
N:	1617
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	COUP is a multi-faceted study of X-ray emission from young stars in the Orion Nebula region based on a nearly continuous 10 day observation conducted by the Chandra X-ray Observatory in January 2003. Maps in 2005ApJS..160..319G, figs 10.
in source:	NAME Orion Nebula
Ref:	=2005ApJS..160..319G
by	GETMAN K.V. , FLACCOMIO E., BROOS P.S., GROSSO N., TSUJIMOTO M., TOWNSLEY L., GARMIRE G.P., KASTNER J., LI J., HARNDEN F.R.Jr, WOLK S., MURRAY S.S., LADA C.J., MUENCH A.A., McCAUGHREAN M.J., MEEUS G., DAMIANI F., MICELA G., SCIORTINO S., BALLY J., HILLENBRAND L.A., HERBST W., PREIBISCH T., FEIGELSON E.D.
	Astrophys. J., Suppl. Ser., 160, 319-352 (2005)
	Chandra Orion Ultradeep Project: observations and sources lists.
o	Table 2: <COUP NNNN> (Nos 1-1616) = <COUP JHHMMSS.s+DDMMSS> N=1616.
Ref:	=2005ApJS..160..353G
by	GETMAN K.V. , FEIGELSON E.D., GROSSO N., McCAUGHREAN M.J., MICELA G., BROOS P., GARMIRE G., TOWNSLEY L.
	Astrophys. J., Suppl. Ser., 160, 353-378 (2005)
	Membership of the Orion nebula population from the Chandra Orion Ultradeep Project.
o	Paragr.4.2: <COUP NNNa> (Nos 599a, 599b) added.
=E=	Catalogue in electronic form as J/ApJS/160/319
=E=	Catalogue in electronic form as J/ApJS/160/353
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: Couteau
Couteau	(Couteau)
Note:	Compilation of 23 publications from 1966 to 1993.
*****	Avoid the usage of Couteau, prefer Cou
Details on Acronym: COVET
COVET	(CFHT-Coma and Virgo Exploration for Transients)
Write:	<<COVET -YYMMDDA>>
Object:	Opt. Transient (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	CFHT observations of optical transients in the frame of the Coma and Virgo Exploration for Transients (COVET). Only the first reference with COVET sources is given here.
Ref:	=2009ATel.1936....1K
by	KASLIWAL M.M. , QUIMBY R., VAN KERKWIJK M.H., KULKARNI S.R., HOWELL D.A., BRETON R.
	ATel, 1936, 1-1 (2009)
	Discovery of twenty one optical transients by CFHT-COVET.
o	Table: <COVET-YYMMDDA> N=21.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cowie
Cowie	(Cowie)
Write:	<<Cowie NNN>>
N:	184
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	List from Cowie, Hawaii Active Catalog of HDF. See alos HDFFF catalog in the HDF Flanking Fields.
in source:	NAME HDFN
Ref:	=1999AJ....117..102B
by	BARGER A.J. , COWIE L.L., TRENTHAM N., FULTON E., HU E.M., SONGAILA A., HALL D.
	Astron. J., 117, 102-110 (1999)
	Constraints on the early formation of field elliptical galaxies.
o	cowie catalog: <Cowie NNN> (Nos 0-183). hff catalog: <HDFFF MMSSs-MMSS> N=2579.
=E=	Catalogue in electronic form as J/AJ/117/102
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cowie
Cowie	(Cowie)
*****	Avoid the usage of Cowie, prefer HDFFF
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [COZ2009]
[COZ2009]	(Casares+Orosz+Zurita+, 2009)
Write:	<<[COZ2009] A>>
N:	5
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	ESO Danish 1.54m telescope DFOSC observations. N=5 local standards in the field of BW Cir.
Ref:	=2009ApJS..181..238C
by	CASARES J. , OROSZ J.A., ZURITA C., SHAHBAZ T., CORRAL-SANTANA J.M., McCLINTOCK J.E., GARCIA M.R., MARTINEZ-PAIS I.G., CHARLES P.A., FENDER R.P., REMILLARD R.A.
	Astrophys. J., Suppl. Ser., 181, 238-243 (2009)
	Refined orbital solution and quiescent variability in the black hole transient GS 1354-64 (= BW cir).
o	Fig.1, Table 1: <[COZ2009] A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CP
CP	(Cape obs., Photographic)
====>	Equivalent to: CPD
Details on Acronym: CP
CP	(Catalog of Pairs)
*****	Avoid the usage of CP, prefer KPG
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CP
CP	(Catalog of Pairs)
*****	Avoid the usage of CP, prefer KPG
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CP
CP	(Cambridge obs., Pulsar)
Rem:	Superseded by PSR
*****	Avoid the usage of CP, prefer PSR
Details on Acronym: [CP2005]
[CP2005]	(Comeron+Pasquali, 2005)
Write:	<<[CP2005] NN>>
N:	19
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Visible and NIR spectroscopy at the Calar Alto 2.2m telescope of stars selected from the 2MASS all-sky-survey in the North America and Pelican nebulae region.
Ref:	=2005A&A...430..541C
by	COMERON F. , PASQUALI A.
	Astron. Astrophys., 430, 541-548 (2005)
	The ionizing star of the North America and Pelican nebulae.
o	Table 1: <[CP2005] NN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 4CP
4CP	(4th Cambridge catalog, Pencil beam fluxes)
Write:	<<4CP DD.NN.N>>
N:	1551
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1966C4CP..C......0C
by	CASWELL J.L.
	The 4CP survey., 0-None (1966)
	The angular structure of radio sources observed at 178 Mc/s. The 4CP survey.
o	<4CP DD.NN.N> N=1551.
Details on Acronym: [CP83]
[CP83]	(Crampton+Parmar, 1983)= ([CP83a])
Write:	<<[CP83] HHMM.m+DDd>>
N:	80
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Note:	See also [CR82], [CSC85], [CC87], [CCH87], [CCS88], [CCH90], [CCH91], [CCH92], [CGC97]
Ref:	=1983PASP...95..127C
by	CRAMPTON D. , PARMAR P.
	Publ. Astron. Soc. Pac., 95, 127-132 (1983)
	Quasar candidates near A 1139, A 1775 and 1633+33.
o	The numbering 'NN' in col(1) of tables is not used in SIMBAD
o	Tables II-IV: <[CP83] HHMM.m+DDd> N=80
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CP83a]
[CP83a]	(Crampton+Parmar, 1983)
*****	Avoid the usage of [CP83a], prefer [CP83]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CP83b]
[CP83b]	(Carruthers+Page, 1983)= (Gru) = (Aqr) (Not yet in Simbad)
Write:	<<[CP83b] Gru C NN>> <<[CP83b] Gru NC NN>> <<[CP83b] Aqr C NN>> <<[CP83b] Aqr NC NN>>
N:	17+23+30+22
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Note:	Table 3A: format 'Gru C NN', objects in Grus field, listed in the Catalog (letter 'C' in the format), N=17 Table 3B: format 'Gru NC NN', objects in Grus field, Not listed in the Catalog (letters 'NC' in the format), N=23 Table 4A: format 'Aqr C NN', objects in Aqr field, listed in the Catalog (letter 'C' in the format), N=30 Table 4B: format 'Aqr NC NN', objects in Aqr field, Not listed in the Catalog (letters 'NC' in the format), N=22
Ref:	=1983ApJS...53..623C
by	CARRUTHERS G.R. , PAGE T.
	Astrophys. J., Suppl. Ser., 53, 623-642 (1983)
	The S 201 far-ultraviolet imaging survey. I. Two fields at high galactic latitude.
o	Table 3A: <[CP83b] Gru C NN> (Nos 1-17). Table 3B: <[CP83b] Gru NC NN> (Nos 1-23). Table 4A: <[CP83b] Aqr C NN> (Nos 1-30). Table 4B: <[CP83b] Aqr NC NN> (Nos 1-22).
Details on Acronym: [CP88]
[CP88]	(Campbell+Persson, 1988)
Write:	<<[CP88] NGC 7538 IRS 3 Star A>>
N:	4
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table III: N=4 * (Nos A-D) in the region of '[WBN74] NGC 7538 IRS 3'
in source:	NGC 7538:[WBN74] NGC 7538 IRS 3 = [WBN74] NGC 7538 IRS 3
Ref:	=1988AJ.....95.1185C
by	CAMPBELL B. , PERSSON S.E.
	Astron. J., 95, 1185-1196 (1988)
	Images of star-forming regions. III. Sources in the NGC 7538 molecular cloud complex.
o	Tables II, III: <[WBN74] NGC 7538 IRS NA> (Nos 2A-2C, 3A-3B, 9A-9D). Table III: <[CP88] NGC 7538 IRS 3 Star A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CP89]
[CP89]	(Caldwell+Phillips, 1989)= (NK)
Write:	<<[CP89] Cl* NNN>> <<[CP89] Star NN>> <<[CP89] NK N>>
N:	121+15+5
Object:	Cluster of * + * + Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 1: N=121 Cl, format 'Cl NNN' Tables 2,3: N=15 * (Nos 3-17), format 'Star NN' Table 4: N=5 Nuclear Knot, format 'NK N'
in source:	NGC 5253
Ref:	=1989ApJ...338..789C
by	CALDWELL N. , PHILLIPS M.M.
	Astrophys. J., 338, 789-803 (1989)
	Star formation in NGC 5253.
o	Table 1: <[CP89] Cl* NNN> (Nos 1-121), Tables 2,3: <[CP89] Star NN> (Nos 3-17), Table 4: <[CP89] NK N> (Nos 1-5)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CP98]
[CP98]	(Coe+Pightling, 1998)
Write:	<<[CP98] RX J1838.4-0301 A>>
N:	12
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Objects inside the error circle of RX J1838.4-0301 Finding chart.
Ref:	=1998MNRAS.299..223C
by	COE M.J. , PIGHTLING S.L.
	Mon. Not. R. Astron. Soc., 299, 223-228 (1998)
	Deep infrared and optical studies of the fields of three proposed TZO remnants.
o	Fig1, Table 1: Objects are [FHR82] A or [FHR82] RN.
o	Fig2, Table 2: <[DAB78] 2S 0142+614 NNa> (No. 2a) and N=5 among (Nos 14-30) added. Fig3, Table 3: <[CP98] RX J1838.4-0301 A> (Nos A-M), No. I missing.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPA2000]
[CPA2000]	(Clocchiatti+PUC+Arevalo+, 2000)
Write:	<<[CPA2000] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of SN 2000FP.
Ref:	=2000IAUC.7549R...1C
by	CLOCCHIATTI A. , PUC-PADOVA SUPERNOVA SEARCH, AREVALO P., RADA C., BARRIENTOS F., MINNITI D., COURBIN F., TURATTO M., ALTAVILLA G., BENETTI S., CAPPELLARO E., PASTORELLO A., LEIBUNDGUT B., SPYROMILIO J.
	IAU Circ., 7549, 1-None (2000)
	Supernova 2000fp in anonymous galaxy.
o	<[CPA2000] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPA2001]
[CPA2001]	(Cichowolski+Pineault+Arnal+, 2001)
Write:	<<[CPA2001] Ring>> <<[CPA2001] GLL.ll+B.bb>> <<[CPA2001] JHHMM+DDMM>> <<[CPA2001] JHHMMSS.ss+DDMMSS.s>>
N:	1+2+1+3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio images of the field around WR 130.
Ref:	=2001AJ....122.1938C
by	CICHOWOLSKI S. , PINEAULT S., ARNAL E.M., TESTORI J.C., GOSS W.M., CAPPA C.E.
	Astron. J., 122, 1938-1953 (2001)
	A DRAO and VLA investigation of the environment of WR 130.
o	Text: <[CPA2001] Ring> N=1, <[CPA2001] JHHMMSS.ss+DDMMSS.s> N=2. Table 3: <[CPA2001] GLL.ll+B.bb> N=1, <[CPA2001] JHHMM+DDMM> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPA2002]
[CPA2002]	(Cappa+Pineault+Arnal+, 2002)
Write:	<<[CPA2002] N>> <<[CPA2002] Structure A>>
N:	7+3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	DRAO Synthesis Telescope observations. N=7 small diameter radio-sources (Nos 1-7). N=3 HI regions.
Ref:	=2002A&A...395..955C
by	CAPPA C. , PINEAULT S., ARNAL E.M., CICHOWOLSKI S.
	Astron. Astrophys., 395, 955-967 (2002)
	An HI interstellar bubble linked to the O-type stars BD +24°3866 and BD +25°3952.
o	Fig.9, Table 3: <[CPA2002] N> (Nos 1-7). Table 6: <[CPA2002] Structure A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPA2006]
[CPA2006]	(Churchwell+Povich+Allen+, 2006)
Write:	<<[CPA2006] WNNN>>
N:	134+188
Object:	Bubble (SIMBAD class: Bubble)
Stat:	is completely incorporated in Simbad
Note:	Images of the GLIMPSE survey have revealed 322 partial and closed rings proposed to represent partially or fully enclosed three-dimensional bubbles.
Ref:	=2006ApJ...649..759C
by	CHURCHWELL E. , POVICH M.S., ALLEN D., TAYLOR M.G., MEADE M.R., BABLER B.L., INDEBETOUW R., WATSON C., WHITNEY B.A., WOLFIRE M.G., BANIA T.M., BENJAMIN R.A., CLEMENS D.P., COHEN M., CYGANOWSKI C.J., JACKSON J.M., KOBULNICKY H.A., MATHIS J.S., MERCER E.P., STOLOVY S.R., UZPEN B., WATSON D.F., WOLFF M.J.
	Astrophys. J., 649, 759-778 (2006)
	The bubbling galactic disk.
o	Table 2: <[CPA2006] WNNN> (Nos N1-N134). Table 3: <[CPA2006] WNNN> (Nos S1-S188).
=E=	Catalogue in electronic form as J/ApJ/649/759
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CPASJ3
CPASJ3	(Catalogue of Photoelectric Astrolabe at San Juan, 3rd) (Not yet in Simbad)
Write:	<<CPASJ3 NNNN>>
N:	6762
Object:	* (SIMBAD class: Star)
Note:	Cooperation between Beijing, San Juan and La Plata observatories.
Ref:	=2005A&A...430..327L
by	LU L.Z. , MANRIQUE W.T., PERDOMO R., WANG Z.Z., PODESTA R.C., ACTIS E.L., ZENG F.M., ALONSO E., ZHAO G., PACHECO A.M., QIAO Q.Y., WANG H.Q.
	Astron. Astrophys., 430, 327-330 (2005)
	Third San Juan photoelectric astrolabe catalogue (CPASJ3).
o	Catalogue: <CPASJ3 NNNN> (Nos 1-6762).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CPB2005]
[CPB2005]	(Chen+Prochaska+Bloom+, 2005)
Write:	<<[CPB2005] host G>> <<[CPB2005] GRB 050730 abs N.NNN>> <<[CPB2005] GRB 050730 abs N.NNNN>> <<[CPB2005] GRB 050730 abs N.NNNNN>>
N:	1+4
Object:	G + Absorber
Note:	Observations of GRB 050730 spectra with the MIKE spectrograph on the Magellan Clay telescope at Las Campanas observatory.
Ref:	=2005ApJ...634L..25C
by	CHEN H.-W. , PROCHASKA J.X., BLOOM J.S., THOMPSON I.B.
	Astrophys. J., 634, 25-28 (2005)
	Echelle spectroscopy of a γ-ray burst afterglow at z = 3.969: a new probe of the interstellar and intergalactic media in the young Universe.
o	Text: <[CPB2005] Host G> N=1. Text: <[CPB2005] GRB 050730 abs N.NNN>, <[CPB2005] GRB 050730 abs N.NNNN>, <[CPB2005] GRB 050730 abs N.NNNNN> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPB2015]
[CPB2015]	(Croxall+Pogge+Berg+, 2015)= ([CPB2015a])
Write:	<<[CPB2015] NGC5194+xxx.x+yyy.y>>
N:	64
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	LBT MODS observations of N=64 HI regions in NGC 5194, as part of the CHemical Abundances Of Spirals (CHAOS) project. See also [BSC2015] for HII regions in NGC 628, [CPB2016] for HII regions in NGC 5457, [BPS2020] for HII regions in NGC 3184, and [RSP2021] for HII regions in NGC 2403.
in source:	M 51 = NGC 5194
Ref:	=2015ApJ...808...42C
by	CROXALL K.V. , POGGE R.W., BERG D.A., SKILLMAN E.D., MOUSTAKAS J.
	Astrophys. J., 808, 42 (2015)
	CHAOS II. Gas-phase abundances in NGC 5194.
o	Table 2: <[CPB2015] NGC5194+xxx.x+yyy.y> N=64.
=E=	Catalogue in electronic form as <J/ApJ/808/42/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [CPB2015a]
[CPB2015a]	(Berg+Skillman+Croxall+, 2015)
*****	Avoid the usage of [CPB2015a], prefer [CPB2015]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [CPB2015b]
[CPB2015b]	(Comerford+Pooley+Barrows+, 2015)
Write:	<<[CPB2015b] JHHMM+DDMMWW>>
N:	24
Object:	AGN (SIMBAD class: AGN = Active Galaxy Nucleus)
Note:	Chandra ACIS and HST WFC3 observations of N=24 X-ray sources in 12 SDSS dual AGN candidates.
Ref:	=2015ApJ...806..219C
by	COMERFORD J.M. , POOLEY D., BARROWS R.S., GREENE J.E., ZAKAMSKA N.L., MADEJSKI G.M., COOPER M.C.
	Astrophys. J., 806, 219 (2015)
	Merger-driven fueling of active galactic nuclei: six dual and offset AGNs discovered with Chandra and Hubble Space Telescope observations.
o	Fig. 3, Tables 4+7: <[CPB2015b] JHHMM+DDMMWW> N=24+20.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPB2016]
[CPB2016]	(Croxall+Pogge+Berg+, 2016)
Write:	<<[CPB2016] NGC 5457+xxx.x+yyy.y>>
N:	102
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	LBT MODS observations of N=102 HII regions in NGC 5457, as part of the CHemical Abundances Of Spirals (CHAOS) project. See also [BSC2015] for HII regions in NGC 628, [CPB2015] for HII regions in NGC 5194, [BPS2020] for HII regions in NGC 3184, and [RSP2021] for HII regions in NGC 2403.
in source:	M 101 = NGC 5457
Ref:	=2016ApJ...830....4C
by	CROXALL K.V. , POGGE R.W., BERG D.A., SKILLMAN E.D., MOUSTAKAS J.
	Astrophys. J., 830, 4-4 (2016)
	CHAOS III: gas-phase abundances in NGC 5457.
o	Table 2: <[CPB2016] NGC 5457+xxx.x+yyy.y> N=102.
=E=	Catalogue in electronic form as <J/ApJ/830/4/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPB2018]
[CPB2018]	(Contreras+Phillips+Burns+, 2018)
Write:	<<[CPB2018] NNN>>
N:	25
Object:	* (SIMBAD class: Star)
Note:	Swift UVOT, LCO 1-m Swope telescope, La Silla TAROT (Telescope a Action Rapide pour les Objets Transitoires), LCO du Pont 2.5-m telescope observations of N=25local sequence stars in the field of SN 2012fr. Use of La Silla-QUEST (LSQ) Low Redshift Supernova Survey data. Use of observations with the 0.5-m Slooh Space robotic telescope at Mt Teide, Tenerife. Use of Backyard Observatory Supernova Search (BOSS) data.
Ref:	=2018ApJ...859...24C
by	CONTRERAS C. , PHILLIPS M.M., BURNS C.R., PIRO A.L., SHAPPEE B.J., STRITZINGER M.D., BALTAY C., BROWN P.J., CONSEIL E., KLOTZ A., NUGENT P.E., TURPIN D., PARKER S., RABINOWITZ D., HSIAO E.Y., MORRELL N., CAMPILLAY A., CASTELLON S., CORCO C., GONZALEZ C., KRISCIUNAS K., SERON J., TUCKER B.E., WALKER E.S., BARON E., CAIN C., CHILDRESS M.J., FOLATELLI G., FREEDMAN W.L., HAMUY M., HOEFLICH P., PERSSON S.E., SCALZO R., SCHMIDT B., SUNTZEFF N.B.
	Astrophys. J., 859, 24-24 (2018)
	SN 2012fr: ultraviolet, optical, and near-infrared light curves of a Type Ia supernova observed within a day of explosion.
o	Tables 2+9: <[CPB2018] NNN> N=25 among (Nos 1-103).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CPC
CPC	(Cape obs., Photographic Catalog)= (CZ) = (CZC)
Write:	<<CPC NN NNNNN>> <<CPC NN.N NNNN>>
N:	86794
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	In the format, the first 2 digits stands for the volume number, NN.N stands for the volume number and the part in the volume 21.
Ref:	=1954AnCap..17...40J
by	JACKSON J. , STOY R.H.
	Ann. Cape Obs., 17, 40-None (1954)
	Cape Photographic Catalogue for 1950.0, zone -30 to -35.
o	<CPC vv NNNNN>
Ref:	=1955AnCap..18....0J
by	JACKSON J. , STOY R.H.
	Ann. Cape Obs., -1-None (1955)
	Cape Photographic Catalogue for 1950.0, zone -35 to -40.
o	<CPC vv NNNNN>
Ref:	=1955AnCap..19....0J
by	JACKSON J. , STOY R.H.
	Ann. Cape Obs., -1-None (1955)
	Cape Photographic Catalogue for 1950.0, zone -52 to -56.
o	<CPC vv NNNNN>
Ref:	=1958AnCap..20....0J
by	JACKSON J. , STOY R.H.
	Ann. Cape Obs., -1-None (1958)
	Cape Photographic Catalogue for 1950.0, zone -56 to -64.
o	<CPC vv NNNNN>
Ref:	=1966AnCap..21....0S
by	STOY R.H.
	Ann. Cape Obs., -1-None (1966)
	Cape Photographic Catalogue for 1950.0, zone -64 to -80.
o	<CPC vv.n NNNN>
Ref:	=1968AnCap..22....0S
by	STOY R.H.
	Ann. Cape Obs., -1-None (1968)
	Cape Photographic Catalogue for 1950.0, zone -80 to -90.
o	<CPC vv NNNNN>
=E=	Catalogue in electronic form as I/5
=E=	Catalogue in electronic form as I/116
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CPC
CPC	(Chopped Photometric Channel)
*****	Avoid the usage of CPC, prefer [VDD93]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CPC2
CPC2	(Cape Photograhic Catalogue 2)
Write:	<<CPC2 FFNNNN>>
N:	266629+8040
Object:	* (SIMBAD class: Star)
Note:	Final catalogue of the CPC2: N=266629 in the main catalogue + N=8040 stars added in appendix.
Ref:	=1984MNRAS.208..911N
by	NICHOLSON W. , PENSTON M.J., MURRAY C.A., DE VEGT C.
	Mon. Not. R. Astron. Soc., 208, 911-923 (1984)
	Second Cape Photographic Catalogue 1950.0 - I - Provisional catalogue of positions of stars in the Cape Zone, -40 to -52 °.
o	<CPC2 FFNNNN>
Ref:	=1999AJ....117.2895Z
by	ZACHARIAS N. , ZACHARIAS M.I., DE VEGT C.
	Astron. J., 117, 2895-2901 (1999)
	The second Cape photographic catalogue on the Hipparcos system.
o	<CPC2 FFNNNN> N=2666629+8040.
=E=	Catalogue in electronic form as I/85
=E=	Catalogue in electronic form as I/265
Details on Acronym: [CPC2008]
[CPC2008]	(Cooksey+Prochaska+Chen+, 2004)
Write:	<<[CPC2008] QSO J1305-1033 abs N.NNNNN>> <<[CPC2008] NNNN>>
N:	28+3542
Object:	ALS + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Las Campanas Observatory du Pont telescope spectroscopy of the field surrounding PKS 1302-102. Archival HST STIS and FUSE spectra of PKS 1302-102.
Ref:	=2008ApJ...676..262C
by	COOKSEY K.L. , PROCHASKA J.X., CHEN H.-W., MULCHAEY J.S., WEINER B.J.
	Astrophys. J., 676, 262-285 (2008)
	Characterizing the low-redshift intergalactic medium toward PKS 1302-102.
o	Tables 3, 7, 10: <[CPC2008] QSO J1305-1033 abs N.NNNNN> N=28. Table 8: <[CPC2008] NNNN> (Nos 1-3542).
=E=	Catalogue in electronic form as J/ApJ/676/262
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CPD
CPD	(Cape obs., Photographic Durchmusterung)= CP = DM
Write:	<<CPD -DD NNNNNA>>
N:	454875
Object:	* (SIMBAD class: Star)
Ref:	=1896AnCap...3....1G
by	GILL D. , KAPTEYN J.C.
	Ann. Cape Obs., 3, 1-None (1896)
	Cape photographic Durchmusterung for the equinox 1875 (-18 to -37).
o	<CPD -DD NNNNN>
Ref:	=1897AnCap...4....1G
by	GILL D. , KAPTEYN J.C.
	Ann. Cape Obs., 4, 1-None (1897)
	Cape photographic Durchmusterung for the equinox 1875 (-38 to -52).
o	<CPD -DD NNNNN>
Ref:	=1900AnCap...5....1G
by	GILL D. , KAPTEYN J.C.
	Ann. Cape Obs., 5, 1-None (1900)
	Cape photographic Durchmusterung for the equinox 1875 (-53 to -89).
o	<CPD -DD NNNNN>
Ref:	=1903AnCap...9....1G
by	GILL D.
	Ann. Cape Obs., 9, 1-None (1903)
	Revision of the Cape photographic Durchmusterung for the equinox 1875.
o	<CPD -DD NNNNN>
=E=	Catalogue in electronic form as I/108
Details on Acronym: [CPE99]
[CPE99]	(Choi+Panis+Evans II, 1999)
Write:	<<[CPE99] IRAS 20050+2720 A>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio map of IRAS 20050+2720 (Fig.16a) shows 4 peaks, called A to D. See also [CTG97]
in source:	IRAS 20050+2720
Ref:	=1999ApJS..122..519C
by	CHOI M. , PANIS J.-F., EVANS II N.J.
	Astrophys. J., Suppl. Ser., 122, 519-556 (1999)
	Berkeley-Illinois-Maryland association survey of protostellar collapse candidates in HCO^+ and HCN lines.
o	Fig.2: Sources A, B, C are respectively [JCC87] IRAS 4A, [JCC87] IRAS 4B, and [JCC87] IRAS 4B2, in SIMBAD.
o	Fig.9, Table 3: <[CED93] 4E> N=1 added. Fig.16, Table 3: <[CPE99] IRAS 20050+2720 A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPF2008]
[CPF2008]	(Comeron+Pasquali+Figueras+, 2008)
Write:	<<[CPF2008] NNN>>
N:	236
Object:	* in Assoc. (SIMBAD class: Star)
Note:	Calar Alto 1.23m and 2.2m telescopes MAGIC and CAFOS observations of the Cygnus OB2 association. Additional use of 2MASS archival data.
in source:	Ass Cyg OB 2 = NAME VI CYG
Ref:	=2008A&A...486..453C
by	COMERON F. , PASQUALI A., FIGUERAS F., TORRA J.
	Astron. Astrophys., 486, 453-466 (2008)
	The outskirts of Cygnus OB2.
o	Tables 1-9: <[CPF2008] NNN> N=236 among (Nos 1-250).
=E=	Catalogue in electronic form as J/A+A/486/453
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPF2015]
[CPF2015]	(Cadelano+Pallanca+Ferraro+, 2015)
Write:	<<[CPF2015] COM-47TucA>>
N:	8
Object:	WD* (SIMBAD class: WhiteDwarf = White Dwarf)
Note:	HST WFC3 photometric observations of N=8 optical white dwarf companions to binary millisecond pulsars (MSP) in the globular cluster 47 Tucanae. See also [RVH2015].
in source:	NGC 104 = 47 Tuc
Ref:	=2015ApJ...812...63C
by	CADELANO M. , PALLANCA C., FERRARO F.R., SALARIS M., DALESSANDRO E., LANZONI B., FREIRE P.C.C.
	Astrophys. J., 812, 63 (2015)
	Optical identification of He white dwarfs orbiting four millisecond pulsars in the globular cluster 47 Tucanae.
o	Table 2: <[CPF2015] COM-47TucA> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPF88]
[CPF88]	(Cesaroni+Palagi+Felli+, 1988)
Write:	<<[CPF88] HHMMSS.s+DDMMSS.s>>
N:	526+13
Object:	H2O Maser (SIMBAD class: Maser)
Note:	Table I: N=526 galactic masers. Table II: N=13 extragalactic sources
Ref:	=1988A&AS...76..445C
by	CESARONI R. , PALAGI F., FELLI M., CATARZI M., COMORETTO G., DI FRANCO S., GIOVANARDI C., PALLA F.
	Astron. Astrophys., Suppl. Ser., 76, 445-458 (1988)
	A catalogue of H2O maser sources north of δ = -30.
o	Tables I, II: <[CPF88] HHMMSS.s+DDMMSS.s> N=526+13
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CPG
CPG	(Catalog of Pairs of G)
*****	Avoid the usage of CPG, prefer KPG
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CPG
CPG	(Catalog of Pairs of G)
*****	Avoid the usage of CPG, prefer KPG
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CPG
CPG	(Catalog Principal of Galaxies)
*****	Avoid the usage of CPG, prefer LEDA
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CPG2019]
[CPG2019]	(Chen+Pineda+Goodman+, 2019)
Write:	<<[CPG2019] L1688-aNNW>> <<[CPG2019] B18-dN>>
N:	12+5+6
Object:	Dense core + Poss. Dense Core (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	N=12+6 gravitationally unbound and pressure confined coherent structures ("droplets") in LDN 1688 and Barnard 18 respectively, and N=5 candidates, using Green Bank Ammonia Survey (GAS) 23GHz NH3 data.
in source:	NAME RHO OPH CLOUD:LDN 1688 = LDN 1688
in source:	NAME Taurus Cloud:Barnard 18 = Barnard 18
Ref:	=2019ApJ...877...93C
by	CHEN H.H.-H. , PINEDA J.E., GOODMAN A.A., BURKERT A., OFFNER S.S.R., FRIESEN R.K., MYERS P.C., ALVES F., ARCE H.G., CASELLI P., CHACON-TANARRO A., CHEN M.C.-Y., DI FRANCESCO J., GINSBURG A., KEOWN J., KIRK H., MARTIN P.G., MATZNER C., PUNANOVA A., REDAELLI E., ROSOLOWSKY E., SCIBELLI S., SEO Y., SHIRLEY Y., SINGH A., (The GAS Collaboration)
	Astrophys. J., 877, 93-93 (2019)
	Droplets. I. Pressure-dominated coherent structures in L1688 and B18.
o	Figs 1-6, Table 1: <[CPG2019] L1688-aNW> (Nos d1-d12, c1E-c1W, c2-c5), <[CPG2019] B18-dN> (Nos d1-d6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CPGA
CPGA	(Catalogue of Southern Peculiar G)
**	catalog: use AM
Details on Acronym: [CPH93]
[CPH93]	(Courtes+Petit+Hua+, 1993)
Write:	<<[CPH93] NNAa>>
N:	139
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	In the format 'NNAa', 'Aa' stands for fields: N (North) (Nos 1N-9N, 5Na-5Nb)), C or Ca and Cb (Center) (Nos 1C-84C), S or Sa (South) N=28 among (Nos 2S-33S) and (Nos 1Sa-10Sa) with No. 9Sa missing. Charts Plates A-E
in source:	NGC 4258
Ref:	=1993A&A...268..419C
by	COURTES G. , PETIT H., HUA C.T., MARTIN P., BLECHA A., HUGUENIN D., GOLAY M.
	Astron. Astrophys., 268, 419-442 (1993)
	Structure of the spiral arms of NGC 4258 in H-α and at 2000A.
o	<[CPH93] NNAa> N=137
Ref:	=1999Ap&SS.263..135C
by	CASTELLANOS M. , DIAZ A.I., TERLEVICH H., GARCIA-VARGAS M.L.
	Astrophys. Space Sci., 263, 135-138 (1999)
	Spectrophotometric analysis of HII regions in NGC 4258.
o	Table 1: HII regions (Nos 2A-2D) not identified.
o	Table 1: <[CPH93] 5Na> (Nos 5Na-5Nb) added.
=E=	Catalogue in electronic form as J/A+A/268/419
=E=	Catalogue in electronic form as J/A+AS/131/317
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPH99]
[CPH99]	(Cole+Pedlar+Holloway+, 1999)
Write:	<<[CPH99] A>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	MERLIN observations of Mrk 273. N=3 continuum radio components A to C. See also [KLY97].
in source:	Mrk 273
Ref:	=1999MNRAS.310.1033C
by	COLE G.H.J. , PEDLAR A., HOLLOWAY A.J., MUNDELL C.G.
	Mon. Not. R. Astron. Soc., 310, 1033-1038 (1999)
	Neutral gas and dust in the central region of the ultraluminous infrared galaxy Mrk273.
o	Table 1: absorption components 'Aa'and 'BN' not in SIMBAD.
o	Fig.1, Table 1: <[CPH99] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPI2007]
[CPI2007]	(CHapman+Penarrubia+Ibata+, 2007)
Write:	<<[CPI2007] JHHMMSS.ss+DDMMSS.s>>
N:	8
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Keck II DEIMOS observations of And XII. N=8 stars associated with And XII.
Ref:	=2007ApJ...662L..79C
by	CHAPMAN S.C. , PENARRUBIA J., IBATA R., McCONNACHIE A., MARTIN N., IRWIN M., BLAIN A., LEWIS G.F., LETARTE B., LO K., LUDLOW A., O'NEIL K.
	Astrophys. J., 662L, 79-82 (2007)
	Strangers in the night: discovery of a dwarf spheroidal galaxy on its first Local Group infall.
o	Table 1: <[CPI2007] JHHMMSS.ss+DDMMSS.s> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPK2001]
[CPK2001]	(Campusano+Pello+Kneib+, 2001)
Write:	<<[CPK2001] ENN>> <<[CPK2001] VNN>> <<[CPK2001] Central Clump>> <<[CPK2001] Clump N>>
N:	5+18+1+2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Study of the field of ACCG 114. Fig.1: (Nos E1-E5) are added to [NKS98] numbering, and 18 new background galaxies (Nos V1-V18). N=1 Central Clump and N=2 Clumps, components of ACCG 114. See also [SCE95] and [NKS98].
in source:	ACCG 114 = ACO S 1077
Ref:	=2001A&A...378..394C
by	CAMPUSANO L.E. , PELLO R., KNEIB J.-P., LE BORGNE J.-F., FORT B., ELLIS R., MELLIER Y., SMAIL I.
	Astron. Astrophys., 378, 394-407 (2001)
	VLT spectroscopy of galaxies lensed by the AC 114 cluster: Implications for the mass model and the study of low-luminosity galaxies at high-redshift.
o	Table 2: Objects which are not [CPK2001] VNN are [NKS98] AN in SIMBAD.
o	Figs 1, 5, Table 2: <[NKS98] AN> (Nos E1-E5) = [CPK2001] EN> (Nos E1-E5). Table 2: <[CPK2001] VNN> (Nos V1-V18). Table 4: <[CPK2001] Central Clump> N=1, <[CPK2001] Clump N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPK2007]
[CPK2007]	(Carpano+Pollock+King+, 2007)= ([CPK2007a])
Write:	<<[CPK2007] SSS>>
N:	1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton discovery of a Super Soft Source (SSS) in NGC 4631.
in source:	NGC 4631
Ref:	=2007A&A...471L..55C
by	CARPANO S. , POLLOCK A.M.T., KING A.R., WILMS J., EHLE M.
	Astron. Astrophys., 471L, 55-58 (2007)
	An ultraluminous supersoft source with a 4-hour modulation in NGC 4631.
o	Table 1, Fig.4, paragraph 4. NGC 4361 is a probable misprint for NGC 4631.
o	Text: <[CPK2007] SSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPK2007a]
[CPK2007a]	(Carpano+Pollock+King+, 2007)
*****	Avoid the usage of [CPK2007a], prefer [CPK2007]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPK2007b]
[CPK2007b]	(Ciechanowska+Pietrzynski+Kolaczkowski+, 2007)
Write:	<<[CPK2007b] NNNNN>> <<[CPK2007b] VNN.N>>
Object:	* + V* (SIMBAD class: Star)
Note:	Search for V* in NGC 6755 with the Warsaw 1.3m telescope at Las Campanas Observatory.
in source:	NGC 6755
Ref:	=2007AcA....57..249C
by	CIECHANOWSKA A. , PIETRZYNSKI G., KOLACZKOWSKI Z., WYRZYKOWSKI L., SZEWCZYK O., KUBIAK M., UDALSKI A., SZYMANSKI M.K.
	AcA, 57, 249-266 (2007)
	The Optical Gravitational Lensing Experiment. Variable stars in the field of open cluster NGC 6755.
o	Table 2: <[CPK2007b] NNNNN> (Nos 1-16595). Table 3: <[CPK2007b] VNN.N> (Nos V1-V9, V10.1-V10.2, V11-V33). Table 4: <[CPK2007b] VNN> (Nos 31-34). Table 5: <[CPK2007b] VNN> (Nos 35-42). Table 6: <[CPK2007b] VNN> (Nos 43-70).
=E=	Catalogue in electronic form as J/AcA/57/249
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPK2013]
[CPK2013]	(Chang+Protopapas+Kim+, 2013) (Not yet in Simbad)
Write:	<<[CPK2013] JHHMMSS+DDMMSS>> <<[CPK2013] DSNNNN>>
N:	1578
Object:	delta Scuti * (SIMBAD class: delSctV* = delta Sct Variable)
Note:	Catalog of N=1578 δ Scuti stars.
Ref:	=2013AJ....145..132C
by	CHANG S.-W. , PROTOPAPAS P., KIM D.-W., BYUN Y.-I.
	Astron. J., 145, 132 (2013)
	Statistical properties of Galactic δ Scuti stars: revisited.
o	Table 3: <[CPK2013] DSNNNN> (Nos DS1-DS1578) = <[CPK2013] JHHMMSS+DDMMSS> N=1578.
o	Table 5: ID M13-V47 not identified (not enough information).
=E=	Catalogue in electronic form as <J/AJ/145/132/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPK2018]
[CPK2018]	(Campos+Pelisoli+Kamann+, 2018)
Write:	<<[CPK2018] NN>>
N:	30
Object:	* (SIMBAD class: Star)
Note:	Photometry of N=30 stars in the globular cluster 47 Tucanae. Use of archival HST WFC3/UVIS images.
in source:	NGC 104 = 47 Tuc
Ref:	=2018MNRAS.481.4397C
by	CAMPOS F. , PELISOLI I., KAMANN S., HUSSER T.-O., DREIZLER S., BELLINI A., ROBINSON E.L., NARDIELLO D., PIOTTO G., KEPLER S.O., ISTRATE A.G., WINGET D.E., MONTGOMERY M.H., DOTTER A.
	Mon. Not. R. Astron. Soc., 481, 4397-4409 (2018)
	Outliers: multicolour photometry guiding the search for evolved binary systems in the globular cluster 47 Tucanae.
o	Table 1: <[CPK2018] NN> (Nos 1-30).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPL2008]
[CPL2008]	(Capelato+Proust+Lima Neto+, 2008)
Write:	<<[CPL2008] NNN>>
N:	128
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ESO 3.6m EFOSC spectroscopy of galaxies in the field of ACO 1942.
in source:	ACO 1942
Ref:	=2008A&A...492..345C
by	CAPELATO H.V. , PROUST D., LIMA NETO G.B., SANTOS W.A., SODRE L.Jr
	Astron. Astrophys., 492, 345-354 (2008)
	The structure and dynamics of Abell 1942.
o	Fig.2: The mentionned arc was previously cited by Smail et al. (1991MNRAS.252...19S)
o	Table A.1: <[CPL2008] NNNN> (Nos 1-128).
=E=	Catalogue in electronic form as J/A+A/492/345
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CPM
CPM	(Campbell+Persson+Matthews)
Write:	<<CPM NN>> <<CPM PNN>> <<CPM HHMMm+DDMM A>>
N:	40+18
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	Search for YSO associated with IRAS. Table I: N=40 YSO, (Nos 1-40), some IRAS corresponding to several YSO format 'HHMMm+DDMM A'. Table III: N=18 Possible YSO, (Nos P1-P18) See also Paper I: [PC87], and Paper II: [PC88]
Ref:	=1989AJ.....98..643C
by	CAMPBELL B. , PERSSON S.E., MATTHEWS K.
	Astron. J., 98, 643-658 (1989)
	Identification of new young stellar objects associated with IRAS point sources. III. The Northern Galactic Plane.
o	Fig.1: The reference stars named 'Star A' in some charts are not in SIMBAD.
o	Table I: <CPM NN> (Nos 1-40), <CPM HHMMm+DDMM A>. Table III: <CPM PNN> (Nos P1-P18).
Origin	of the Acronym: L (1998AJ....116..868I)
Details on Acronym: [CPM2012]
[CPM2012]	(CLOSE+PUGLISI+MALES+, 2012)
Write:	<<[CPM2012] JHHMMSS.sss+DDMMSS.sss>> <<[CPM2012] AN>>
N:	47
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	LBT adaptive secondary AO system observations of the Orion Trapezium cluster.
in source:	NAME Ori Trapezium
Ref:	=2012ApJ...749..180C
by	CLOSE L.M. , PUGLISI A., MALES J.R., ARCIDIACONO C., SKEMER A., GUERRA J.C., BUSONI L., BRUSA G., PINNA E., MILLER D.L., RICCARDI A., McCARTHY D.W., XOMPERO M., KULESA C., QUIROS-PACHECO F., ARGOMEDO J., BRYNNEL J., ESPOSITO S., MANNUCCI F., BOUTSIA K., FINI L., THOMPSON D.J., HILL J.M., WOODWARD C.E., BRIGUGLIO R., RODIGAS T.J., BRIGUGLIO R., STEFANINI P., AGAPITO G., HINZ P., FOLLETTE K., GREEN R.
	Astrophys. J., 749, 180 (2012)
	High-resolution images of orbital motion in the Orion Trapezium cluster with the LBT AO system.
o	Table 1: <[CPM2012] JHHMMSS.sss+DDMMSS.sss> N=47.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPO2009]
[CPO2009]	(Chauhan+Pandey+Ogura+, 2009)
Write:	<<[CPO2009] NNN>> <<[CPO2009] JHHMMSS.ss+DDMMSS.s>> <<[CPO2009] JHHMMSS.s+DDMMSS>>
N:	133+419
Object:	* + Poss. YSO (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	2m Himalayan Chandra Telescope and 1.04m Sampurnanand Telescope observations of stars in bright-rimmed clouds. Use of archival data from 2MASS and Spitzer IRAC.
Ref:	=2009MNRAS.396..964C
by	CHAUHAN N. , PANDEY A.K., OGURA K., OJHA D.K., BHATT B.C., GHOSH S.K., RAWAT P.S.
	Mon. Not. R. Astron. Soc., 396, 964-983 (2009)
	Triggered star formation and evolution of T-Tauri stars in and around bright-rimmed clouds.
o	Tables 3-4: <[CPO2009] NNN> (Nos 1-133). Tables 6-7: <[CPO2009] JHHMMSS.ss+DDMMSS.s>, <[CPO2009] JHHMMSS.s+DDMMSS>, N=420.
=E=	Catalogue in electronic form as J/MNRAS/396/964
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPO2011]
[CPO2011]	(Chauhan+Pandey+Ogura+, 2011)
Write:	<<[CPO2011] NNN>>
N:	247
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Note:	Kiso 1.05-m, ARIES 1.04-m Sampurnanand telescope, Himalayan Chandra 2-m telescope (HCT) observations of N=247 YSOs in the W 5E HII region.
in source:	W 5:W 5E = W 5E
in source:	SFO 13
in source:	SFO 14
in source:	[NTI2009] cloud 4
Ref:	=2011MNRAS.415.1202C
by	CHAUHAN N. , PANDEY A.K., OGURA K., JOSE J., OJHA D.K., SAMAL M.R., MITO H.
	Mon. Not. R. Astron. Soc., 415, 1202-1219 (2011)
	Star formation in bright-rimmed clouds and clusters associated with the W5 E H II region.
o	Table 3: <[CPO2011] NNN> (Nos 1-247).
=E=	Catalogue in electronic form as J/MNRAS/415/1202
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CPOC
CPOC	(COMPLETE Perseus Outflow Candidate)
Write:	<<CPOC NN>>
N:	60
Object:	Poss. Outflow (SIMBAD class: Outflow_Candidate = Outflow Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=60 outflow candidates in the Perseus Molecular Cloud. Use of 12CO(1-0) and 13CO(1-0) data from the COordinated Molecular Probe Line Extinction Thermal Emission (COMPLETE) Survey of Star Forming Regions (see http://www.cfa-harvard.edu/COMPLETE).
in source:	NAME Perseus Molecular Cloud
Ref:	=2010ApJ...715.1170A
by	ARCE H.G. , BORKIN M.A., GOODMAN A.A., PINEDA J.E., HALLE M.W.
	Astrophys. J., 715, 1170-1190 (2010)
	The complete survey of outflows in Perseus.
o	Table 1: <CPOC NN> (Nos 1-60).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CPR2000]
[CPR2000]	(Cappellaro+Pastorello+Rizzi+, 2000)
Write:	<<[CPR2000] JHHMMSS.ss+DDMMSS.s>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host G of SN 1999GT and SN 1999GU.
Ref:	=2000IAUC.7346R...1C
by	CAPPELLARO E. , PASTORELLO A., RIZZI L., SALVO M., TURATTO M., DANZIGER J., MAZZALI P., PATAT F., BENETTI S., LEISY P., POMPEI E.
	IAU Circ., 7346, 1-None (2000)
	Supernovae 1999gt and 1999gu.
o	<[CPR2000] JHHMMSS.ss+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPR2002]
[CPR2002]	(Comeron+Pasquali+Rodighiero+, 2002)
Write:	<<[CPR2002] {A\|B\|C}NN>>
N:	46+20+3
Object:	* in Assoc. (SIMBAD class: Star)
Note:	Calar Alto observations. Table 1: Early-type stars. Table 2: * with Br-gamma in emission. Table 3: * with CO in emission.
in source:	Ass Cyg OB 2 = NAME VI CYG
Ref:	=2002A&A...389..874C
by	COMERON F. , PASQUALI A., RODIGHIERO G., STANISHEV V., DE FILIPPIS E., LOPEZ-MARTI B., GALVEZ-ORTIZ M.C., STANKOV A., GREDEL R.
	Astron. Astrophys., 389, 874-888 (2002)
	On the massive star contents of Cygnus OB2.
o	Table 1: <[CPR2002] ANN> (Nos A1-A46). Table 2: <[CPR2002] ANN> (Nos B1-B20). Table 4: <[CPR2002] AN> (Nos C1-C3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CPS
CPS	(COMPLETE Perseus Shell)
*****	Avoid the usage of CPS, prefer [ABG2011]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CPS2000]
[CPS2000]	(Clocchiatti+Phillips+Suntzeff+, 2000)= (92ar)
Write:	<<[CPS2000] A>> <<[CPS2000] NN>>
N:	3+14
Object:	G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Objects in the field of SN 1992AR. (Nos A-C) are galaxies. (Nos 1-14) are photometric standards, except 4 which are also galaxies.
Ref:	=2000ApJ...529..661C
by	CLOCCHIATTI A. , PHILLIPS M.M., SUNTZEFF N.B., DELLA VALLE M., CAPPELLARO E., TURATTO M., HAMUY M., AVILES R., NAVARRETE M., SMITH C., RUBENSTEIN E.P., COVARRUBIAS R., STETSON P.B., MAZA J., RIESS A.G., ZANIN C.
	Astrophys. J., 529, 661-674 (2000)
	The luminous type Ic Supernova 1992ar at z=0.145.
o	Fig.1: <[CPS2000] A> (Nos A-C). Fig.1, Table 3: <[CPS2000] N> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPS2005]
[CPS2005]	(Chand+Petitjean+Srianand+, 2005)
Write:	<<[CPS2005] QSO JHHMM+DDMM abs N.NNN>>
N:	33
Object:	Absorber
Note:	VLT UVES sample of 17 QSOs spectra with 33 absorption systems.
Ref:	=2005A&A...430...47C
by	CHAND H. , PETITJEAN P., SRIANAND R., ARACIL B.
	Astron. Astrophys., 430, 47-58 (2005)
	Probing the time-variation of the fine-structure constant: Results based on Si IV doublets from a UVES sample.
o	Table 1: <[CPS2005] QSO JHHMM+DDMM abs N.NNN> N=33.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPS2006]
[CPS2006]	(Chies-Santos+Pastoriza+Santiago+, 2006)= ([CPS2006a])
Write:	<<[CPS2006] DDD.ddddddd+DD.ddddddd>>
N:	777
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	Use of archival HST WFPC2 images to search for globular clusters in NGC 5846.
in source:	NGC 5846
Ref:	=2006A&A...455..453C
by	CHIES-SANTOS A.L. , PASTORIZA M.G., SANTIAGO B.X., FORBES D.A.
	Astron. Astrophys., 455, 453-459 (2006)
	The globular cluster system of NGC5846 revisited: colours, sizes and X-ray counterparts.
o	Table 3: <[CPS2006] DDD.ddddddd+DD.ddddddd> N=777.
=E=	Catalogue in electronic form as J/A+A/455/453
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPS2006a]
[CPS2006a]	(Chies-Santos+Pastoriza+Santiago+, 2006)
*****	Avoid the usage of [CPS2006a], prefer [CPS2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPS2006b]
[CPS2006b]	(Coppolani+Petitjean+Stoehr+, 2006) (Not yet in Simbad)
Write:	<<[CPS2006b] QSO JHHMM+DDMM abs N.NN>> <<[CPS2006b] QSO JHHMM+DDMM abs N.NNN>>
N:	29
Object:	Absorber
Ref:	=2006MNRAS.370.1804C
by	COPPOLANI F. , PETITJEAN P., STOEHR F., ROLLINDE E., PICHON C., COLOMBI S., HAEHNELT M.G., CARSWELL B., TEYSSIER R.
	Mon. Not. R. Astron. Soc., 370, 1804-1816 (2006)
	Transverse and longitudinal correlation functions in the intergalactic medium from 32 close pairs of high-redshift quasars.
o	Appendix: <[CPS2006b] QSO JHHMM+DDMM abs N.NN>, <[CPS2006b] QSO JHHMM+DDMM abs N.NNN>, N=29.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPS2011]
[CPS2011]	(Carrera+Page+Stevens+, 2011)
Write:	<<[CPS2011] NNN>> <<[CPS2011] Blob>>
N:	10+1
Object:	(smm) + (Rad) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Use of optical, infrared and radio data to study the structure around a QSO. See also [SPI2004].
Ref:	=2011MNRAS.413.2791C
by	CARRERA F.J. , PAGE M.J., STEVENS J.A., IVISON R.J., DWELLY T., EBRERO J., FALOCCO S.
	Mon. Not. R. Astron. Soc., 413, 2791-2807 (2011)
	A strongly star-forming group: three massive galaxies associated with a quasi-stellar object.
o	Fig. 1, Tables 1, 3-4: <[CPS2011] NNN> N=10 among (nos 13-512). Table 4: <[CPS2011] Blob> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPS2012]
[CPS2012]	(Chen+Peng+Strom+, 2012)= ([CPS2012a])
Write:	<<[CPS2012] NN>>
N:	18
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	NAOC Xinglong Station 2.16m telescope spectroscopy of N=18 galaxies in the field of 4C 73.08.
Ref:	=2012MNRAS.422.3004C
by	CHEN R. , PENG B., STROM R.G., WEI J.
	Mon. Not. R. Astron. Soc., 422, 3004-3009 (2012)
	Group of galaxies around the giant radio galaxy 4C 73.08.
o	Fig. 3, Tables 1-2: <[CPS2012] NN> (Nos 1-18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPS2012a]
[CPS2012a]	(Chen+Peng+Strom+, 2012)
*****	Avoid the usage of [CPS2012a], prefer [CPS2012]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPS2012b]
[CPS2012b]	(Chen+Peng+Strom+, 2012)
Write:	<<[CPS2012b] NN>>
N:	60
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	NAOC Xinglong Station 2.16m telescope spectroscopy of N=60 galaxies in the field of the giant radio galaxy NGC 315.
Ref:	=2012MNRAS.420.2715C
by	CHEN R. , PENG B., STROM R.G., WEI J.
	Mon. Not. R. Astron. Soc., 420, 2715-2726 (2012)
	Galaxy group around giant radio galaxy NGC 315.
o	Tables 1-2: <[CPS2012b] NN> (Nos 1-60).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPS85]
[CPS85]	(Caux+Puget+Serra+, 1985)
Write:	<<[CPS85] LLL.l+BB.b>>
N:	58
Object:	(Far IR) (SIMBAD class: Infrared = Infra-Red Source)
Ref:	=1985A&A...144...37C
by	CAUX E. , PUGET J.L., SERRA G., GISPERT R., RYTER C.E.
	Astron. Astrophys., 144, 37-48 (1985)
	Far-infrared survey of the galactic disc. II. The sources.
o	<[CPS85] LLL.l+BB.b> N=58
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPS87]
[CPS87]	(Courtes+Petit+Sivan+, 1987)
*****	Avoid the usage of [CPS87], prefer CPSDP
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPS88]
[CPS88]	(Campbell+Persson+Strom+, 1988)
Write:	<<[CPS88] Knot N>> <<[CPS88] Star A>>
N:	6+4
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=6 knots in the jet of SSV LDN 1551 5 and N=4 stars in the field.
in source:	LDN 1551:SSV LDN 1551 5 = SSV LDN 1551 5
Ref:	=1988AJ.....95.1173C
by	CAMPBELL B. , PERSSON S.E., STROM S.E., GRASDALEN G.L.
	Astron. J., 95, 1173-1184 (1988)
	Images of star-forming regions. II. The circumstellar environment of L 1551 IRS 5.
o	L 1551 IRS 5 = SSV LDN 1551 5 in Simbad.
o	Table II: <[CPS88] Knot N> (Nos 1-6), <[CPS88] Star A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPS95]
[CPS95]	(Colbert+Petre+Schlegel+, 1995)
Write:	<<[CPS95] X-NNA>>
N:	12+1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	PSPC and IPC ROSAT observations. See also [SPC2000].
in source:	NGC 1313
Ref:	=1995ApJ...446..177C
by	COLBERT E.J.M. , SCHLEGEL E.M., RYDER S.D.
	Astrophys. J., 446, 177-193 (1995)
	Soft X-ray emission from the spiral galaxy NGC 1313.
o	<[CPS95] X-NN> (Nos X-1 to X-10)
Ref:	=1998AJ....116.1657M
by	MILLER S. , SCHLEGEL E.M., PETRE R., COLBERT E.
	Astron. J., 116, 1657-1670 (1998)
	X-ray properties of NGC 1313: second-epoch PSPC observations.
o	Fig.1b, Tables, text: <[CPS95] X-NNA> (Nos X-11, X-12, X-1A) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CPSDP
CPSDP	(Courtes+Petit+Sivan+Dodonov+Petit)= [CPS87] = (Z)
Write:	<<CPSDP NNNA>>
N:	456
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Table 2: first part of the table, (Nos among 1-1502) are BCLMP objects. Objects named Z NNNA by the authors, (Nos 1-410), N=456, are CPSDP objects.
in source:	M 33 = NGC 598
Ref:	=1987A&A...174...28C
by	COURTES G. , PETIT H., SIVAN J.P., DODONOV S., PETIT M.
	Astron. Astrophys., 174, 28-56 (1987)
	H-α survey of M 33 with the six-meter telescope: morphology of the general diffuse emission, evidence for a chaotic medium of bubbles and filaments.
o	First part of table 2: (Nos among 1-1502) are BCLMP obj. Col. (3): cross-id LMA
o	Table 2: <CPSDP NNNA> N=456 among (Nos 1-410, 1A-366A).
=E=	Catalogue in electronic form as J/A+AS/131/317
Origin	of the Acronym: L (1997PASP..109..927W)
Details on Acronym: [CPV2011]
[CPV2011]	(Calvi+Poggianti+Vulcani, 2011)= (PM2GC)
Write:	<<[CPV2011] GRPM2 NNNN>> <<[CPV2011] GRNNNN>> (not recognised by Simbad, but found in literature)
N:	176
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	N=176 galaxy groups in the Padova-Millenium Galaxy and Group Catalogue (PM2GC), using galaxies from the Millenium Galaxy Catalogue (MGC).
Ref:	=2011MNRAS.416..727C
by	CALVI R. , POGGIANTI B.M., VULCANI B.
	Mon. Not. R. Astron. Soc., 416, 727-738 (2011)
	The Padova–Millennium galaxy and group catalogue (PM2GC): the group-finding method and the PM2GC catalogues of group, binary and single field galaxies.
o	Table 2: <[CPV2011] GRPM2 NNNN> N=176 among (Nos 1000-1230).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPV99]
[CPV99]	(Corradi+Perinotto+Villaver+, 1999) (Not yet in Simbad)
Write:	<<[CPV99] NGC 3918 A>> <<[CPV99] NGC 3918 A'>> <<[CPV99] NGC 3918 A">> <<[CPV99] K 1-2 A>> <<[CPV99] K 1-2 A'>> <<[CPV99] Wray 17-1 A>> <<[CPV99] Wray 17-1 A'>>
N:	6+2+6
Object:	Component of PN (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST and NTT images of 3 PN.
in source:	NGC 3918
in source:	PN K 1-2
in source:	WRAY 17-1
Ref:	=1999ApJ...523..721C
by	CORRADI R.L.M. , PERINOTTO M., VILLAVER E., MAMPASO A., GONCALVES D.R.
	Astrophys. J., 523, 721-733 (1999)
	Jets, knots, and tails in planetary nebulae: NGC 3918, K1-2, and Wray 17-1.
o	Table 2, Fig.1: <[CPV99] NGC 3918 A> (Nos A-C), <[CPV99] NGC 3918 A'> (No. A'), <[CPV99] NGC 3918 A"> (No. A"). Fig.6: <[CPV99] K 1-2 A> (No. A), <[CPV99] K 1-2 A'> (No. A'). Fig.8: <[CPV99] Wray 17-1 A> (Nos A-D), <[CPV99] Wray 17-1 A'> (Nos A', B').
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPW2007]
[CPW2007]	(Carpano+Pollock+Wims+, 2007)
Write:	<<[CPW2007] NGC 300 X-N>>
N:	1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of NGC 300. The source NGC X-1 is a good candidate for a WR-Black Hole X-ray binary.
in source:	NGC 300
Ref:	=2007A&A...461L...9C
by	CARPANO S. , POLLOCK A.M.T., WILMS J., EHLE M., SCHIRMER M.
	Astron. Astrophys., 461L, 9-12 (2007)
	A Wolf-Rayet/black-hole X-ray binary candidate in NGC 300.
o	<[CPW2007] NGC 300 X-N> (No. X-1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CPW2010]
[CPW2010]	(Chen+Perley+Wilson+, 2010)
Write:	<<[CPW2010] GRB 080607 host G>>
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Multiwavelength imaging observations of GRB 080607 host galaxy.
Ref:	=2010ApJ...723L.218C
by	CHEN H.-W. , PERLEY D.A., WILSON C.D., CENKO S.B., LEVAN A.J., BLOOM J.S., PROCHASKA J.X., TANVIR N.R., DESSAUGES-ZAVADSKY M., PETTINI M.
	Astrophys. J., 723L, 218-222 (2010)
	A mature dusty star-forming galaxy hosting GRB 080607 at z = 3.036.
o	(Erratum) erratum vol. 723, p. L53 (2010)
o	<[CPW2010] GRB 080607 host G> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 7CQ
7CQ	(7C catalog, QSO)
Write:	<<7CQ HHMM+DDdA>>
N:	204+26
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Note:	Tables 1, 2: Selection of candidate radio-loud QSOs from the 7C survey. Format used by the authors is 'HHMM+DDd', a letter A, B, C is added when there is more than one optically unresolved object in the field of the radio-source.
Ref:	=1999MNRAS.307..293R
by	RILEY J.M. , RAWLINGS S., McMAHON R.G., BLUNDELL K.M., MILLER P., LACY M., WALDRAM E.M.
	Mon. Not. R. Astron. Soc., 307, 293-314 (1999)
	Quasars from the 7C survey _ I. Sample selection and radio maps.
o	Tables 1, 2: <7CQ HHMM+DDdA> N=204+26.
=E=	Catalogue in electronic form as <J/MNRAS/307/293/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CQZ2019]
[CQZ2019]	(Cao+Qiu+Zhang+, 2019)
Write:	<<[CQZ2019] CNNW-N>> <<[CQZ2019] DRNNWN-NN>> <<[CQZ2019] WNNN-N>> <<[CQZ2019] WNNNWN-N>> <<[CQZ2019] WWNNW-N>> <<[CQZ2019] W75N-N>>
N:	151
Object:	Dense Core (SIMBAD class: denseCore = Dense Core)
Note:	N=151 massive dense cores in the Cygnus X molecular complex, using infrared to (sub)millimeter data from Spitzer, Herschel, the JCMT, and the IRAM 30m telescope.
in source:	NAME Cyg X
Ref:	=2019ApJS..241....1C
by	CAO Y. , QIU K., ZHANG Q., WANG Y., HU B., LIU J.
	Astrophys. J., Suppl. Ser., 241, 1-1 (2019)
	Surveys of clumps, cores, and condensations in Cygnus X. I. A new catalog of ~0.1 pc massive dense cores.
o	Tables 6-9: <[CQZ2019] CNNW-N>, <[CQZ2019] DRNNWN-NN, <[CQZ2019] WNNN-N>, <[CQZ2019] WNNNWN-N>, <[CQZ2019] WWNNW-N>, N=151.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Cr
Cr	(Crowther) (Not yet in Simbad)
Write:	<<Cr ?>>
N:	562
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Ph. D. Dissertation, Univ. Cambridge, England, 1966, Crowwther. High resolution observations at a wavelength of 1.7 metres.
Auth.:	CROWTHER J.H.
Details on Acronym: Cr
Cr	(Collinder)
*****	Avoid the usage of Cr, prefer Collinder
Details on Acronym: CR
CR	(Chandler+Richer)
*****	Avoid the usage of CR, prefer [CR2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CR
CR	(Chincarini+Rood)
*****	Avoid the usage of CR, prefer [CR71]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CR
CR	(Ciatti+Rosino)
*****	Avoid the usage of CR, prefer [CR77]
Origin	of the Acronym: L (1998ApJ...509...80S)
Details on Acronym: [CR2000]
[CR2000]	(Chandler+Richer, 2000)= (CR) = ([CR2000a])
Write:	<<[CR2000] N>>
N:	2
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SCUBA observations. N=2 Sub-millimeter continuum peaks in [JCC87] IRAS 2.
in source:	NGC 1333:[JCC87] IRAS 2 = [JCC87] IRAS 2
Ref:	=2000ApJ...530..851C
by	CHANDLER C.J. , RICHER J.S.
	Astrophys. J., 530, 851-866 (2000)
	The structure of protostellar envelopes derived from submillimeter continuum images.
o	IRAS 2 = [JCC87] IRAS 2.
o	<[CR2000] N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CR2000a]
[CR2000a]	(Chandler+Richer, 2000)
Note:	N=2 Sub-millimeter continuum peaks in [JCC87] IRAS 2.
*****	Avoid the usage of [CR2000a], prefer [CR2000]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CR2000b]
[CR2000b]	(Cooke+Reid, 2000)
Write:	<<[CR2000b] NNNNN>>
N:	189
Object:	PM* (SIMBAD class: HighPM* = High Proper Motion Star)
Note:	PM* in Kapteyn SA 94, selected in a catalogue of N=27748 objects.
in source:	SA 94-
Ref:	=2000MNRAS.318.1206C
by	COOKE J.A. , REID I.N.
	Mon. Not. R. Astron. Soc., 318, 1206-1216 (2000)
	High proper motion stars in Kapteyn Selected Area 94.
o	Table 2: <[CR2000b] NNNNN> N=189 among 27748.
=E=	Catalogue in electronic form as J/MNRAS/318/1206
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CR2010]
[CR2010]	(Curtis+Richer, 2010) (Not yet in Simbad)
Write:	<<[CR2010] JHHMMSS.ss+DDMMSS.s>>
N:	85+122
Object:	Clump (SIMBAD class: denseCore = Dense Core)
Note:	N=85+122 star-forming cores in the Perseus molecular cloud. Use of SCUBA 850µm data.
in source:	NAME Perseus Molecular Cloud
Ref:	=2010MNRAS.402..603C
by	CURTIS E.I. , RICHER J.S.
	Mon. Not. R. Astron. Soc., 402, 603-619 (2010)
	The properties of SCUBA cores in the Perseus molecular cloud: the bias of clump-finding algorithms.
o	Tables A1-A2: <[CR2010] JHHMMSS.ss+DDMMSS.s> N=85+122.
=E=	Catalogue in electronic form as J/MNRAS/402/603
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 3CR
3CR	(3rd Cambridge catalog, Revised)
Write:	<<3CR NNN.N>>
N:	328
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Revised version of the 3C catalogue based on new observations. Objects already in the 3C catalogue have the same number 'NNN' sometimes written 'NNN.0' in the literature. Some sources are omitted on account of errors in the original 3C list. New sources added have a format 'NNN.N', derived from the 3C NNN source preceding it in R.A. See also [SDM85].
Ref:	=1962MmRAS..68..163B
by	BENNETT A.S.
	Mem. R. Astron. Soc., 68, 163-None (1962)
	The revised 3C catalogue of radio sources.
o	Catalogue: <3CR NNN>, <3CR NNN.N>, N=328.
Ref:	=1985PASP...97..932S
by	SPINRAD H. , DJORGOVSKI S., MARR J., AGUILAR L.
	Publ. Astron. Soc. Pac., 97, 932-961 (1985)
	A third update of the status of the 3 CR sources: further new redshifts and new identifications of distant galaxies.
o	Catalogue: <3CR NNN.N> N=293, <[SDM85] 3CR NNNA> (Nos 66A-66B, 225A-225B, 292).
=E=	Catalogue in electronic form as VIII/1
Details on Acronym: [CR71]
[CR71]	(Chincarini+Rood, 1971)= (CR)
Write:	<<[CR71] NN>>
N:	47
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	NAME Perseus Cluster
Ref:	=1971ApJ...168..321C
by	CHINCARINI G. , ROOD H.J.
	Astrophys. J., 168, 321-325 (1971)
	Dynamics of the Perseus cluster of galaxies.
o	Table 1: <[CR71] NN> (Nos 1-47)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CR77]
[CR77]	(Ciatti+Rosino, 1977)= (CR)
Write:	<<[CR77] NGC NNNN A>> <<[CR77] NGC NNNN a>>
N:	13+10+10+8
Object:	* (SIMBAD class: Star)
Note:	Comparison stars in the fields of SNR host galaxies: NGC 3627, 7495, 4414, 7343. Finding charts.
Ref:	=1977A&A....56...59C
by	CIATTI F. , ROSINO L.
	Astron. Astrophys., 56, 59-64 (1977)
	The type II supernova 1973r in NGC 3627.
o	Table 2: <[CR77] NGC 3627 A> (Nos A-B), <[CR77] NGC 3627 a> (Nos a-i, l, m).
Ref:	=1977A&A....57...73C
by	CIATTI F. , ROSINO L.
	Astron. Astrophys., 57, 73-83 (1977)
	Photographic and spectroscopic observations of four type I SN.
o	Table 2: <[CR77] NGC 7495 a> N=10 among (Nos a-n). Table 4: <[CR77] NGC 4414 A> N=10 among (Nos B-P). Table 7: <[CR77] NGC 7343 a> N=8 among (Nos a-m).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CR78]
[CR78]	(Ciatti+Rosino, 1978)
Write:	<<[CR78] Anon 1512+02 a>> <<[CR78] MCG +FF-FF-NN a>> <<[CR78] NGC NNNN a>>
N:	62
Object:	* (SIMBAD class: Star)
Note:	Asiago systematic study of supernovae. Reference stars in the field of 6 galaxies host of SN
Ref:	=1978A&AS...34..387C
by	CIATTI F. , ROSINO L.
	Astron. Astrophys., Suppl. Ser., 34, 387-402 (1978)
	Observations of ten SN (1973-1977).
o	Fig.1: <[CR78] Anon 1512+02 a> (Nos a-d). Fig.3: <[CR78] MCG +9-23-25 a> (Nos a-i). Fig.6: <[CR78] NGC 7723 a> (Nos a-h). Fig.9: <[CR78] NGC 2487 a> (Nos a-g). Fig.11: <[CR78] NGC 3583 a> (Nos a-h). Fig.12: <[CR78] NGC 3756 a> (Nos a-i, l). Fig.14: <[CR78] NGC 4402 a> (Nos a-i). Fig.16: <[CR78] NGC 977 a> (Nos a-d). Fig.18: <[CR78] MCG +5-26-14 a> (Nos a-c).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CR82]
[CR82]	(Crampton+Rensing, 1982)
Write:	<<[CR82] HHMM.m+DDd>> <<[CR82] HHMM.m+DDMM>>
N:	26
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Note:	See also [CP83], [CSC85], [CC87], [CCH87], [CCS88], [CCH90], [CCH91], [CCH92], [CGC97]
Ref:	=1982PASP...94..440C
by	CRAMPTON D. , RENSING M.
	Publ. Astron. Soc. Pac., 94, 440-443 (1982)
	Quasar candidates near 3C 345.
o	Table I, col.(1): internal numbering 'NN' not used
o	Table I: <[CR82] HHMM.m+DDd>, <[CR82] HHMM.m+DDMM> N=26
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CR86]
[CR86]	(Chan+Richer, 1986)
Write:	<<[CR86] NNNN>>
N:	73
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	CTIO observations. Blink survey to select UV-excess objects in a field centered on M 4. Among the 73 objects in Table 2, 10 are White Dwarf stars, 37 are QSOs, 11 are Galaxies.
Ref:	=1986ApJ...302..257C
by	CHAN E. , RICHER H.B.
	Astrophys. J., 302, 257-271 (1986)
	Ultraviolet-excess objects in the field of NGC 6121 (M 4).
o	Table 2: <[CR86] NNNN> N=73 among (Nos 86-1747).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CR95]
[CR95]	(Combi+Romero, 1995)= ([CR95a])
Write:	<<[CR95] NN>>
N:	30
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
in source:	NAME Ara Region
Ref:	=1995A&A...303..872C
by	COMBI J.A. , ROMERO G.E.
	Astron. Astrophys., 303, 872-880 (1995)
	On the origin of the γ-ray fields in the Ara region.
o	PKS 1610-60 = PKS 1610-607
o	<NAME ARA 335-11>, Table 1: <[CR95] NN> (Nos 1-30)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CR95a]
[CR95a]	(Combi+Romero, 1995)
*****	Avoid the usage of [CR95a], prefer [CR95]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CR95b]
[CR95b]	(Corcoran+Ray, 1995)
Write:	<<[CR95b] V380 Ori-A>>
N:	2
Object:	* (SIMBAD class: Star)
Note:	UKIRT IRCAM observations of N=2 sources near V380 Ori.
Ref:	=1995A&A...301..729C
by	CORCORAN D. , RAY T.P.
	Astron. Astrophys., 301, 729-748 (1995)
	Herbig-Haro outflows in the V380 Orionis region.
o	N3SK50 = KMS 31 (cf. 1989ApJS.71.183S), fig. 4 and 15: knots not in SIMBAD
o	<HH NNN> No. 148. Fig. 11: <[CR95b] V380 Ori-A> (No B-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CR96]
[CR96]	(Cernicharo+Reipurth, 1996) (Not yet in Simbad)
Write:	<<[CR96] bullet N>>
N:	3
Object:	CO bullet (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=3 CO Bullets in the CO flow of HH 111.
in source:	HH 111
Ref:	=1996ApJ...460L..57C
by	CERNICHARO J. , REIPURTH B.
	Astrophys. J., 460, 57-60 (1996)
	Herbig-haro jets, CO flows, and CO bullets: the case of HH 111.
o	IRAS 0591+0247 misprint for IRAS 05491+0247
o	Fig.5, Paragr.4: <[CR96] bullet N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CrA
CrA	(CrA Cloud)
*****	Avoid the usage of CrA, prefer [LEM2005b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CrA
CrA	(CrA Cloud)
*****	Avoid the usage of CrA, prefer Wa
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CRA2005]
[CRA2005]	(Cappellaro+Riello+Altavilla+, 2005)
Write:	<<[CRA2005] J1888-A>> <<[CRA2005] AXAF-A>> <<[CRA2005] 10Z2-A>> <<[CRA2005] 13Z3-A>> <<[CRA2005] Field2-A>>
N:	12+9+3+6+2
Object:	Poss. SN (SIMBAD class: Supernova = SuperNova)
Note:	MPG-ESO 2.2m telescope observations of 21 fields. N=32 SN candidates.
Ref:	=2005A&A...430...83C
by	CAPPELLARO E. , RIELLO M., ALTAVILLA G., BOTTICELLA M.T., BENETTI S., CLOCCHIATTI A., DANZIGER J.I., MAZZALI P., PASTORELLO A., PATAT F., SALVO M., TURATTO M., VALENTI S.
	Astron. Astrophys., 430, 83-93 (2005)
	Death rate of massive stars at redshift ~0.3.
o	Table 2: <[CRA2005] J1888-A> N=12 among (Nos A-Q), <[CRA2005] AXAF-A> (Nos A-J, G missing), <[CRA2005] 10Z2-A> (Nos A-B, D), <[CRA2005] 13Z3-A> N=6 among (Nos A-K), <[CRA2005] Field2-A> (Nos F,G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRA2011]
[CRA2011]	(Cusano+Ripepi+Alcala+, 2011)
Write:	<<[CRA2011] D25 JHHMMSSss+DDMMSS.s>>
N:	5
Object:	H-alpha Em* (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Note:	VLT VIMOS observations of the star-forming complex Sh 2-284.
in source:	SH 2-284
Ref:	=2011MNRAS.410..227C
by	CUSANO F. , RIPEPI V., ALCALA J.M., GANDOLFI D., MARCONI M., DEGL'INNOCENTI S., PALLA F., GUENTHER E.W., BERNABEI S., COVINO E., NEINER C., PUGA E., HONY S.
	Mon. Not. R. Astron. Soc., 410, 227-240 (2011)
	Pre-main-sequence stars in the star-forming complex sh 2-284.
o	Tables 2-5: <[CRA2011] D25 JHHMMSSss+DDMMSSs> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRA98]
[CRA98]	(Combi+Romero+Arnal, 1998)
Write:	<<[CRA98] NN>>
N:	11
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1998A&A...333..298C
by	COMBI G.E. , ROMERO E.M., ARNAL J.A.
	Astron. Astrophys., 333, 298-304 (1998)
	The spur-like radio feature in Centaurus.
o	p. 303: CLUST 3 = [ME95] CLUST 3
o	Table 1: <[CRA98] NN> (Nos 1-11)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CrAPMS
CrAPMS	(Corona Australis, Pre-Main-Seq. *)
Write:	<<CrAPMS NNWW>>
N:	14
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Einstein IPC observations PMS in the R CrA association. See also Wa, CHX, ScoPMS
in source:	NAME R CrA Cloud
Ref:	=1997AJ....114.1544W
by	WALTER F.M. , VRBA F.J., WOLK S.J., MATHIEU R.D., NEUHAEUSER R.
	Astron. J., 114, 1544-1554 (1997)
	X-ray sources in regions of star formation. VI. The R CrA association as viewed by EINSTEIN.
o	'nTT JHHMMSS+DDMM' designation not in SIMBAD
o	Table 2: <CrAPMS NNWW> (Nos 1-11), N=14
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CRATES
CRATES	(Combined Radio All-Sky Targeted Eight GHz Survey)
Write:	<<CRATES JHHMMSS+DDMMSS>>
N:	about 11000
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	New and archival VLA and ATCA data of flat-spectrum radio sources.
Ref:	=2007ApJS..171...61H
by	HEALEY S.E. , ROMANI R.W., TAYLOR G.B., SADLER E.M., RICCI R., MURPHY T., ULVESTAD J.S., WINN J.N.
	Astrophys. J., Suppl. Ser., 171, 61-71 (2007)
	CRATES: an all-sky survey of flat-spectrum radio sources.
o	Tables 5, 6: <CRATES JHHMMSS+DDMMSS> N=about 11000.
=E=	Catalogue in electronic form as J/ApJS/171/61
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CRB
CRB	(Cowan+Roberts+Branch)
*****	Avoid the usage of CRB, prefer [CB85]
Origin	of the Acronym: L (1994ApJ...434..128C)
Details on Acronym: CRB
CRB	(Corcoran+Ray+Bastein)
Note:	Feature near LkHa 198.
*****	Avoid the usage of CRB, prefer [CRB95]
Origin	of the Acronym: L (1996ApJ...472..349A)
Details on Acronym: [CRB2001]
[CRB2001]	(Combi+Romero+Benaglia+, 2001)= ([CRB2001a]) (Not yet in Simbad)
Write:	<<[CRB2001] CN>>
N:	2
Object:	Cloud (SIMBAD class: Cloud)
Note:	N=2 standard clouds: C1 associated with 3EG J1834-2803, C2 associated with 3EG J1850-2652.
Ref:	=2001A&A...366.1047C
by	COMBI J.A. , ROMERO G.E., BENAGLIA P., JONAS J.L.
	Astron. Astrophys., 366, 1047-1052 (2001)
	Detection of a new, low-brightness supernova remnant possibly associated with EGRET sources.
o	The new SNR is SNR 006.5-12.0
o	<[CRB2001] CN> (Nos C1-C2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRB2001a]
[CRB2001a]	(Combi+Romero+Benaglia+, 2001) (Not yet in Simbad)
*****	Avoid the usage of [CRB2001a], prefer [CRB2001]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRB2001b]
[CRB2001b]	(Combi+Romero+Benaglia+, 2001)
Write:	<<[CRB2001b] SN>>
N:	7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=7 point sources radio-sources near GRO J1655-40. VLA image in Fig.1.
Ref:	=2001A&A...370L...5C
by	COMBI J.A. , ROMERO G.E., BENAGLIA P., MIRABEL I.F.
	Astron. Astrophys., 370, 5-8 (2001)
	The radio surroundings of the microquasar GRO J1655-40.
o	Table 1: <[CRB2001b] SN> (Nos S1-S7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRB2015]
[CRB2015]	(Chene+Ramirez Alegria+Borissova+, 2015)
Write:	<<[CRB2015] VVV CL041-N>> <<[CRB2015] DDD.ddddddd+DD.ddddddd>>
N:	8+221493
Note:	VLT ISAAC and Gemini Flamingos-2 spectroscopy of N=8 stars in the VVV CL041 cluster. N=221493 stars in the photometric catalog. The photometric data used are part of the ESO Public Survey VVV, which observes with the VISTA InfraRed CAMera (VIRCAM) at the VISTA 4m telescope at Paranal Observatory.
in source:	VVV CL041
Ref:	=2015A&A...584A..31C
by	CHENE A.-N. , RAMIREZ ALEGRIA S., BORISSOVA J., O'LEARY E., MARTINS F., HERVE A., KUHN M., KURTEV R., CONSUELO AMIGO FUENTES P., BONATTO C., MINNITI D.
	Astron. Astrophys., 584A, 31-31 (2015)
	Massive open star clusters using the VVV survey. IV. WR 62-2, a new very massive star in the core of the VVVCL041 cluster.
o	Fig. 1, Table 1: <[CRB2015] VVV CL041-N> (Nos 1-8). Catalog: <[CRB2015] DDD.ddddddd+DD.ddddddd> N=221493.
o	WR 62-2 is 2MASS J14462640-5923291 in SIMBAD.
=E=	Catalogue in electronic form as <J/A+A/584/A31/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRB2016]
[CRB2016]	(Carballo-Bello+Ramirez Alegria+Borissova+, 2016)
Write:	<<[CRB2016] NN>> <<[CRB2016] VN>>
N:	10+3
Object:	RR Lyr + * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Magellan Clay telescope and MMT spectroscopic and photometric NIR observations of N=10+3 stars of the globular cluster 2MASS-GC 03. Use of archival VVV survey images.
in source:	NAME 2MASS-GC03
Ref:	=2016MNRAS.462..501C
by	CARBALLO-BELLO J.A. , RAMIREZ ALEGRIA S., BORISSOVA J., SMITH L.C., KURTEV R., LUCAS P.W., MONI BIDIN C., ALONSO-GARCIA J., MINNITI D., PALMA T., DEKANY I., MEDINA N., MOYANO M., VILLANUEVA V., KUHN M.A.
	Mon. Not. R. Astron. Soc., 462, 501-510 (2016)
	Near-infrared photometry and spectroscopy of the low Galactic latitude globular cluster 2MASS-GC 03.
o	Table 1: <[CRB2016] NN> (Nos 1-10). Table 2: <[CRB2016] VN> (Nos (V1-V3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRB2019]
[CRB2019]	(Claeyssens+Richard+Blaizot+, 2019)
Write:	<<[CRB2019] N.Na>>
N:	7+8
Object:	Grav. lensed image (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy)
Note:	VLT MUSE observations of N=7 gravitationally lensed images and N=8 components in the field of the galaxy cluster MCS J0940.9+0744. In the format N.Na, the suffix a refers to the continuum measured on HST (a), and Lyman α peaks labelled (b) and (c).
in source:	MCS J0940.9+0744
Ref:	=2019MNRAS.489.5022C
by	CLAEYSSENS A. , RICHARD J., BLAIZOT J., GAREL T., LECLERCQ F., PATRICIO V., VERHAMME A., WISOTZKI L., BACON R., CARTON D., CLEMENT B., HERENZ E.C., MARINO R.A., MUZAHID S., SAUST R., SCHAYE J.
	Mon. Not. R. Astron. Soc., 489, 5022-5029 (2019)
	Spectral variations of Lyman αemission within strongly lensed sources observed with MUSE.
o	Fig. 1, Table A2: <[CRB2019] MACS 0940 N.N> (Nos 1.1-1.4, 2.1-2.3), <[CRB2019] MACS 0940 N.Na> (Nos 1.1a, 1.2a, 1.3a-1.3c, 1.4a-1.4c).
o	SMACS J2031.8-2046 is a misprint for SMACS J2031.8-4036 ([CRH2012] in Simbad).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRB93]
[CRB93]	(Comeron+Rieke+Burrows+, 1993)
*****	Avoid the usage of [CRB93], prefer CRBR
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRB95]
[CRB95]	(Corcoran+Ray+Bastein, 1995)= (CRB) = (IRS)
Write:	<<[CRB95] Loop A>> <<[CRB95] Knot A>> <<[CRB95] IRS N>>
N:	2+10+2
Object:	Feature (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Feature near LkHa 198. See also [AMB96]
Ref:	=1995A&A...293..550C
by	CORCORAN D. , RAY T.P., BASTIEN P.
	Astron. Astrophys., 293, 550-558 (1995)
	Optical outflows in the vicinity of LkHα 198.
o	See also [AMB96] ref. 1996ApJ...472..349A
o	<[CRB95] Loop A> (Nos A-B), <[CRB95] Knot A> (Nos A-J), <[CRB95] IRS N> (Nos 1-2). Fig.2: <Em* LkHA NNNA> (No. 198B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRB99]
[CRB99]	(Combi+Romero+Benaglia, 1999)
Write:	<<[CRB99] A>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=4 elongated radio features in RX J0852.0-4622 SNR.
in source:	RX J0852.0-4622
Ref:	=1999ApJ...519L.177C
by	COMBI J.A. , ROMERO G.E., BENAGLIA P.
	Astrophys. J., 519, 177-180 (1999)
	Radio detection of the supernova remnant RX J0852.0-4622.
o	Table 1, Fig.1: <[CRB99] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CRBB
CRBB	(McCarthy+Rich+Becker+Butler+)
Write:	<<CRBB N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Palomar 60-inch telescope and CTIO observations. CRBB 1 = PN G359.2-33.5
Ref:	=1991ApJ...371..380M
by	McCARTHY J.K. , RICH R.M., BECKER S.R., BUTLER K., HUSFELD D., GROTH H.G.
	Astrophys. J., 371, 380-386 (1991)
	Echelle spectroscopy of CD -41 13967: the young central star of a new planetary nebula.
o	<CRBB N> (No. 1).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CRBR
CRBR	(Comeron+Rieke+Burrows+Rieke)= ([CRB93]) = (Oph)
Write:	<<CRBR MMSS.s-MMSS>>
N:	93
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	format: offset position relative to RA=16h, Dec=-24 deg. Objects are found numbered 'NN' in 1999AJ....117..469W. See [RR90].
in source:	NAME rho Oph Cloud
Ref:	=1993ApJ...416..185C
by	COMERON F. , RIEKE G.H., BURROWS A., RIEKE M.J.
	Astrophys. J., 416, 185-203 (1993)
	The stellar population in the ρ Ophiuchi cluster.
o	<CRBR MMSS.s-MMSS> N=93. RA = 16H, Dec = -24°
Origin	of the Acronym: L (1997ApJS..112..109B)
Details on Acronym: [CRC2021]
[CRC2021]	(Cooper+Rudie+Chen+, 2021)
Write:	<<[CRC2021] JHHMMSS.ss+DDMMSS.s>>
N:	15
Object:	G (SIMBAD class: Galaxy)
Note:	N=15 galaxies around two Lyman limit systems (LLSs) in the line of sight of QSO J0110-1648, as part of the Cosmic Ultraviolet Baryon Survey (CUBS).
Ref:	=2021MNRAS.508.4359C
by	COOPER T.J. , RUDIE G.C., CHEN H.-W., JOHNSON S.D., ZAHEDY F.S., CHEN M.C., BOETTCHER E., WALTH G.L., CANTALUPO S., COOKSEY K.L., FAUCHER-GIGUERE C.-A., GREENE J.E., LOPEZ S., MULCHAEY J.S., PENTON S.V., PETITJEAN P., PUTMAN M.E., RAFELSKI M., RAUCH M., SCHAYE J., SIMCOE R.A.
	Mon. Not. R. Astron. Soc., 508, 4359-4384 (2021)
	The Cosmic Ultraviolet Baryon Survey (CUBS) IV: The complex multiphase circumgalactic medium as revealed by partial Lyman limit systems.
o	Table 4: <[CRC2021] JHHMMSS.ss+DDMMSS.s> N=15.
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [CRC99]
[CRC99]	(Churchill+Rigby+Charlton+, 1999)
Write:	<<[CRC99] SNN>> <<[CRC99] QSO JHHMM+DDMM abs N.NNNNNN>>
N:	30
Object:	Absorber
Note:	Search for MgII absorbers in 26 HIRES-Keck QSO spectra. z with 6 digits in SIMBAD like in Table 2, truncated to 5 digits in text and Table 3.
Ref:	=1999ApJS..120...51C
by	CHURCHILL C.W. , RIGBY J.R., CHARLTON J.C., VOGT S.S.
	Astrophys. J., Suppl. Ser., 120, 51-75 (1999)
	The population of weak Mg II absorbers. I. A survey of 26 QSO HIRES/Keck Spectra.
o	Table 2: 0958+051 is a misprint for QSO 0958+551.
o	Table 2: <[CRC99] SNN> (Nos S1-S30) = <[CRC99] QSO JHHMM+DDMM abs N.NNNNNN> N=30.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRD2019]
[CRD2019]	(Colombo+Rosolowsky+Duarte-Cabral+, 2019)
Write:	<<[CRD2019] NNNNN>>
N:	85020
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	N=85020 molecular clouds in the Milky Way first quadrant. Use of JCMT CO(3-2) High-Resolution Survey (COHRS) data.
Ref:	=2019MNRAS.483.4291C
by	COLOMBO D. , ROSOLOWSKY E., DUARTE-CABRAL A., GINSBURG A., GLENN J., ZETTERLUND E., HERNANDEZ A.K., DEMPSEY J., CURRIE M.J.
	Mon. Not. R. Astron. Soc., 483, 4291-4340 (2019)
	The integrated properties of the molecular clouds from the JCMT CO(3-2) High-Resolution Survey.
o	Table 1: <[CRD2019] NNNNN> (Nos 0-85019).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRE95]
[CRE95]	(Copet+Rouan+Epchtein, 1995)
Write:	<<[CRE95] HHMMSS.s+DDMMSS.s>>
N:	9
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	DENIS survey The authors give no format, so we use coodinates as format
in source:	NAME Orion Nebula
Ref:	=1995MmSAI..66..577C
by	COPET E. , ROUAN D., EPCHTEIN N.
	Mem. Soc. Astron. Ital., 66, 577-584 (1995)
	A near-infrared study of the Orion Nebula with DENIS.
o	Table 1: <[CRE95] HHMMSS.s-DDMMSS.s> N=9
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRF2008]
[CRF2008]	(Chaty+Rahoui+Foellmi+, 2008) (Not yet in Simbad)
Write:	<<[CRF2008] IGR JHHMMm+DDMM CN>>
N:	4+4+4+2+2+4+6+4
Object:	(Near IR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	INTEGRAL observations of hard X-ray sources. Search for candidate counterparts (CN in the format).
Ref:	=2008A&A...484..783C
by	CHATY S. , RAHOUI F., FOELLMI C., TOMSICK J.A., RODRIGUEZ J., WALTER R.
	Astron. Astrophys., 484, 783-800 (2008)
	Multi-wavelength observations of Galactic hard X-ray sources discovered by INTEGRAL. I. The nature of the companion star.
o	Paragraph. 3.1 2MASS J16320215-4752289 is a probable misprint for 2MASS J16320215-4752322.
o	Table 4, Fig.2: <[CRF2008] IGR JHHMMm+DDMM CN> N=4+4+4+2+2+4+6+4.
=E=	Catalogue in electronic form as <J/A+A/484/783/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRG2001]
[CRG2001]	(Cappa+Rubio+Goss, 2001)= ([CRG2001a])
Write:	<<[CRG2001] Cloud A>> <<[CRG2001] W Clump>>
N:	5+2
Object:	Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	CO observations of NGC 2359: N=5 CO emission clouds (Nos A-E). Cloud A consists of 2 clumps E and W. See also [CGN99].
in source:	NGC 2359
Ref:	=2001AJ....121.2664C
by	CAPPA C.E. , RUBIO M., GOSS W.M.
	Astron. J., 121, 2664-2672 (2001)
	CO observations of NGC 2359: the molecular clouds revisited.
o	Fig.2, Table 1: <[CRG2001] Cloud A> (Nos A-E). Text: <[CRG2001] W Clump> (Nos E, W).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRG2001a]
[CRG2001a]	(Cappa+Rubio+Goss, 2001)
*****	Avoid the usage of [CRG2001a], prefer [CRG2001]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRG2001b]
[CRG2001b]	(Clenet+Rouan+Gendron+, 2001)
Write:	<<[CRG2001b] NNa>>
N:	44+2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	RASOIR/ADONIS observations at ESO La Silla. Photometry and astrometry of 44 stars in the Gal Center region.
in source:	NAME Gal Center
Ref:	=2001A&A...376..124C
by	CLENET Y. , ROUAN D., GENDRON E., MONTRI J., RIGAUT F., LENA P., LACOMBE F.
	Astron. Astrophys., 376, 124-135 (2001)
	Adaptive optics L-band observations of the Galactic Center region.
o	Table 2: <[CRG2001b] NNa> (Nos 1-44, 26b-26c).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRG2004]
[CRG2004]	(Clenet+Rouan+Gendron+, 2004)
Write:	<<[CRG2004] NN>>
N:	22
Object:	* in Cl* (SIMBAD class: Star)
Note:	Galactic center observations with NAOS-CONICA at the VLT. N=22 stars members of the Sgr A* Cluster.
in source:	Gal Center:NAME Sgr A* Cluster = NAME Sgr A* Cluster
Ref:	=2004A&A...417L..15C
by	CLENET Y. , ROUAN D., GENDRON E., LACOMBE F., LAGRANGE A.-M., ROUSSET G., GENZEL R., SCHOEDEL R., OTT T., ECKART A., MARCO O., TACCONI-GARMAN L.
	Astron. Astrophys., 417, 15-19 (2004)
	The infrared L'-band view of the Galactic Center with NAOS-CONICA at VLT.
o	OphN9 = [GY92] 232.
o	Table 1: <[CRG2004] NN> (Nos 1-22).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRG2014]
[CRG2014]	(Canning +Ryon+Gallagher+, 2014)
N:	14+1+20 (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST ACS/WFC observations of N=35 star clusters in three outer regions of NGC 1275.
in source:	NGC 1275
Ref:	=2014MNRAS.444..336C
by	CANNING R.E.A. , RYON J.E., GALLAGHER III J.S., KOTULLA R., O'CONNELL R.W., FABIAN A.C., JOHNSTONE R.M., CONSELICE C.J., HICKS A., ROSARIO D., WYSE R.F.G.
	Mon. Not. R. Astron. Soc., 444, 336-349 (2014)
	Filamentary star formation in NGC 1275.
o	Table 3: <[CRG2014] JHHMMSS.s+DDMMSS> N=14+1+20.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRG2019]
[CRG2019]	(Caminha+Rosati+Grillo+, 2019)
Write:	<<[CRG2019] MHHMM-JHHMMSS.ss+DDMMSS.ss>> <<[CRG2019] RHHMM-JHHMMSS.ss+DDMMSS.ss>> <<[CRG2019] MHHMM-NNa>> <<[CRG2019] RHHMM-Na>>
N:	725+236+108+42
Object:	? + Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=725+236 sources and N=108+42 gravitationally lensed images in the field of eight CLASH clusters. Use of HST Cluster Lensing And Supernova survey (CLASH) data, MUSE and CLASH-VLT spectroscopic data.
in source:	ClG J0329-0212 = MCS J0329.7-0212
in source:	ClG J0429-0253 = MCS J0429.6-0253
in source:	MCS J1115.8+0129
in source:	ClG J1311-0311 = MCS J1311.0-0311
in source:	ClG J1931-2635 = MCS J1931.8-2635
in source:	ClG J2129-0741 = MCS J2129.4-0741
in source:	ClG J1347-1145 = RX J1347.5-1145
in source:	RX J2129.6+0005
Ref:	=2019A&A...632A..36C
by	CAMINHA G.B. , ROSATI P., GRILLO C., ROSANI G., CAPUTI K.I., MENEGHETTI M., MERCURIO A., BALESTRA I., BERGAMINI P., BIVIANO A., NONINO M., UMETSU K., VANZELLA E., ANNUNZIATELLA M., BROADHURST T., DELGADO-CORREAL C., DEMARCO R., KOEKEMOER A.M., LOMBARDI M., MAIER C., VERDUGO M., ZITRIN A.
	Astron. Astrophys., 632A, 36-36 (2019)
	Strong lensing models of eight CLASH clusters from extensive spectroscopy: Accurate total mass reconstructions in the cores.
o	Table 2: <[CRG2019] MHHMM-JHHMMSS.ss+DDMMSS.ss> N=725, <[CRG2019] RHHMM-JHHMMSS.ss+DDMMSS.ss> N=236. Table A.2: <[CRG2019] MHHMM-NNa> N=108, <[CRG2019] RHHMM-Na> N=42.
=E=	Catalogue in electronic form as <J/A+A/632/A36/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CRGC
CRGC	(Collisional Ring Galaxy Candidate)
Write:	<<RGC NN>>
N:	25
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 images from the HST archives. Search for Collisional Ring Galaxy Candidates.
Ref:	=2004ApJ...612..679L
by	LAVERY R.J. , REMIJAN A., CHARMANDARIS V., HAYES R.D., RING A.A.
	Astrophys. J., 612, 679-689 (2004)
	Probing the evolution of the galaxy interaction/merger rate using collisional ring galaxies.
o	3C 295 122 is [DG92] 6-122 in Simbad.
o	Table 1: <CRGC NN> (Nos 1-25).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CRH2012]
[CRH2012]	(Christensen+Laursen+Richard+, 2012)
Write:	<<[CRH2012] SMACS JHHMM.m+DDMM>> <<[CRH2012] SMACS JHHMM.m+DDMM N.N>> <<[CRH2012] MACS JHHMM.m+DDMM N.N>> <<[CRH2012] J131132.14-012055.33>>
N:	3+3+3+1
Object:	Cluster of G + Grav. lensed image of a G + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT X-shooter spectroscopy of galaxies strongly lensed by massive galaxy clusters.
Ref:	=2012MNRAS.427.1953C
by	CHRISTENSEN L. , RICHARD J., HJORTH J., MILVANG-JENSEN B., LAURSEN P., LIMOUSIN M., DESSAUGES-ZAVADSKY M., GRILLO C., EBELING H.
	Mon. Not. R. Astron. Soc., 427, 1953-1972 (2012)
	The low-mass end of the fundamental relation for gravitationally lensed star-forming galaxies at 1 < z < 6.
o	<[CRH2012] SMACS JHHMM.m+DDMM> N=3. <[CRH2012] SMACS JHHMM.m+DDMM N.N> N=3. <[CRH2012] MACS JHHMM.m+DDMM N.N> N=3. Paragr. 3.1: <[CRH2012] J131132.14-012055.33> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRH2015]
[CRH2015]	(Chiang+Reipurth+Hillenbrand, 2015)
Write:	<<[CRH2015] JHHMMSS.s+DDMMSS>> <<[CRH2015] NN>>
Object:	* (SIMBAD class: Star)
Note:	Subaru IRCS, UH 2.2m telescope WFGS and Keck I HIRES observations of N=3+22 stars in the vicinity of V1818 Ori. Use of 2MASS, WISE, and ASAS data.
Ref:	=2015AJ....149..108C
by	CHIANG H.-F. , REIPURTH B., HILLENBRAND L.
	Astron. J., 149, 108 (2015)
	The Herbig Be star V1818 Ori and its environment.
o	Table 1: <[CRH2015] JHHMMSS.s+DDMMSS> N=3. Fig. 7, Table 3: <[CRH2015] NN> (Nos 1-22).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Cri
Cri	(Crimee?) (Not yet in Simbad)
*****	Avoid the usage of Cri, prefer [ASV69]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [CRJ2004]
[CRJ2004]	(Cohen+Rottgering+Jarvis+, 2004)
Write:	<<[CRJ2004] JHHMM.m+DDMM>>
N:	949
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA observations, 74MHz survey near the NGP.
Ref:	=2004ApJS..150..417C
by	COHEN A.S. , ROETTGERING H.J.A., JARVIS M.J., KASSIM N.E., LAZIO T.J.W.
	Astrophys. J., Suppl. Ser., 150, 417-430 (2004)
	A deep, high-resolution survey at 74 MHz.
o	Table 2: <[CRJ2004] JHHMM.m+DDMM> N=949.
=E=	Catalogue in electronic form as J/ApJS/150/417
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRK2003]
[CRK2003]	(Cohen+Rottgering+Kassim+, 2003)= (XMM-LSS)
Write:	<<[CRK2003] JHHMM.m+DDMM>> <<[CRK2003] JHHMM.m+DDMMA>>
N:	256+37+211+28
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	XMM Large-Scale Structure Survey (XMM-LSS) is a major project to map the large-scale structure of the Universe, using XMM. Preliminary results from a counterpart VLA 325MHz and a 74MHz survey in a 8degx8deg region. See also [TCR2006], [TRB2007], [TLR2008]
in source:	NAME XMM-LSS Field
Ref:	=2003ApJ...591..640C
by	COHEN A.S. , ROETTGERING H.J.A., KASSIM N.E., COTTON W.D., PERLEY R.A., WILMAN R., BEST P., PIERRE M., BIRKINSHAW M., BREMER M., ZANICHELLI A.
	Astrophys. J., 591, 640-661 (2003)
	The low-frequency radio counterpart of the XMM Large-Scale Structure Survey.
o	Tables 2, 3: <[CRK2003] JHHMM.m+DDMM> N=256+211, <[CRK2003] JHHMM.m+DDMMA> N=37+28.
=E=	Catalogue in electronic form as J/ApJ/591/640
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CRL
CRL	(Cambridge Research Lab.)
Note:	First defined in 1975 by Walter and Price.
====>	Equivalent to: RAFGL
Details on Acronym: [CRM2009]
[CRM2009]	(Cappa+Rubio+Martin+, 2009)
Write:	<<[CRM2009] A>>
N:	3
Object:	(FIR) (SIMBAD class: FarIR = Far-IR source (λ >= 30 µm))
Stat:	is completely incorporated in Simbad
Note:	N=3 extended IR emission regions in the surroundings of WR 55. Use of IRAS HIRES image at 60µm.
Ref:	=2009A&A...508..759C
by	CAPPA C.E. , RUBIO M., MARTIN M.C., ROMERO G.A.
	Astron. Astrophys., 508, 759-771 (2009)
	Unveiling the molecular environment of the ring nebula RCW78.
o	Fig. 9: <[CRM2009] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRM93]
[CRM93]	(Curiel+Rodriguez+Moran+, 1993)
Write:	<<[CRM93] Serpens WW>> <<[CRM93] Knot A>>
N:	3+11
Object:	Lobe + Knot (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	VLA observations. Fig.2: N=3 main components of Serpens Cloud (Nos NW, C, SE) where C stands for Center. N=11 knots in the Serpens radio jet.
in source:	NAME Serpens Cloud
Ref:	=1993ApJ...415..191C
by	CURIEL S. , RODRIGUEZ L.F., MORAN J.M., CANTO J.
	Astrophys. J., 415, 191-203 (1993)
	The triple radio continuum source in Serpens : the birth of a Herbig Haro system ?
o	Fig.2: <[CRM93] Serpens WW> (Nos NW, C, SE), <[CRM93] Knot A> (Nos A-H, X-Z).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRN2020]
[CRN2020]	(Clark+Ritchie+Negueruela, 2020)
Write:	<<[CRN2020] FN>> <<[CRN2020] W1NNN>>
N:	8+69
Object:	Star (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT FLAMES and FORS2 and AAT AAOmega observations of N=69 stars in the Galactic cluster Westerlund 1 and of N=8 field stars.
in source:	Cl Westerlund 1
Ref:	=2020A&A...635A.187C
by	CLARK J.S. , RITCHIE B.W., NEGUERUELA I.
	Astron. Astrophys., 635A, 187-187 (2020)
	A VLT/FLAMES survey for massive binaries in Westerlund 1. VII. Cluster census.
o	Table 2: <[CRN2020] FN> (Nos F1-F8). Table A.1: <[CRN2020] W1NNN> (Nos W1001-W1069).
=E=	Catalogue in electronic form as <J/A+A/635/A187/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRO2009]
[CRO2009]	(Cichowolski+Romero+Ortega+, 2009)
Write:	<<[CRO2009] NN>> <<[CRO2009] Cloud A>> <<[CRO2009] gN>>
Object:	Poss. YSO + Cloud + Group (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Note:	Search for YSO candidates around the HII region Sh 2-173 using MSX6C, 2MASS and IRAS point source catalogs.
in source:	SH 2-173
Ref:	=2009MNRAS.394..900C
by	CICHOWOLSKI S. , ROMERO G.A., ORTEGA M.E., CAPPA C.E., VASQUEZ J.
	Mon. Not. R. Astron. Soc., 394, 900-915 (2009)
	Unveiling the birth and evolution of the HII region Sh2-173.
o	Table 6: <[CRO2009] NN> (Nos 1-46). Fig. 7: <[CRO2009] Cloud A> (Nos A-B). Fig. 9: <[CRO2009] gN> (Nos g1-G4).
=E=	Catalogue in electronic form as J/MNRAS/394/900
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRP2003]
[CRP2003]	(Combi+Romero+Paredes+, 2003)
Write:	<<[CRP2003] J1737-15>> <<[CRP2003] NN>>
N:	23
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA observations of the error box of CGRO EGRET source 3EG J1735-1500. N=23 radio-sources are found, source 10 is a new radio-galaxy 'J1737-15', optical host galaxy observed with Calar Alto telescope.
Ref:	=2003ApJ...588..731C
by	COMBI J.A. , ROMERO G.E., PAREDES J.M., TORRES D.F., RIBO M.
	Astrophys. J., 588, 731-735 (2003)
	Discovery of a new radio galaxy within the error box of the unidentified γ-ray source 3EG J1735-1500.
o	new radio galaxy = [CRP2003] J1737-15
o	<[CRP2003] J1737-15> N=1. Table 1: <[CRP2003] NN> (Nos 1-23).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRR2012]
[CRR2012]	(Combes+Rex+Rawle+, 2012)= (HLS)
Write:	<<[CRR2012] HLS J091828.6+514223>>
N:	1
Object:	smm G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Herschel SPIRE, SMA, IRAM and EVLA observations of N=1 strongly lensed submillimeter galaxy behind the Abell 773 cluster.
in source:	ACO 773
Ref:	=2012A&A...538L...4C
by	COMBES F. , REX M., RAWLE T.D., EGAMI E., BOONE F., SMAIL I., RICHARD J., IVISON R.J., GURWELL M., CASEY C.M., OMONT A., BERCIANO ALBA A., DESSAUGES-ZAVADSKY M., EDGE A.C., FAZIO G.G., KNEIB J.-P., OKABE N., PELLO R., PEREZ-GONZALEZ P.G., SCHAERER D., SMITH G.P., SWINBANK A.M., VAN DER WERF P.
	Astron. Astrophys., 538L, 4-4 (2012)
	A bright z = 5.2 lensed submillimeter galaxy in the field of Abell 773 - HLS J091828.6+514223.
o	<[CRR2012] HLS J091828.6+514223> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRR90]
[CRR90]	(Curiel+Raymond+Rodriguez+, 1990)
Write:	<<[CRR90] L1448N A>> <<[CRR90] L1448C>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=3 radio-sources in LDN 1448, 2 are in LDN 1448North, the other is at the Center ('C' stands for Center)
in source:	LDN 1448
Ref:	=1990ApJ...365L..85C
by	CURIEL S. , RAYMOND J.C., RODRIGUEZ L.F., CANTO J., MORAN J.M.
	Astrophys. J., 365, 85-88 (1990)
	The exciting source of the bipolar outflow in L 1448.
o	Table 1: <[CRR90] L1448N A> (Nos A-B), <[CRR90] L1448C>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRR96]
[CRR96]	(Comeron+Rieke+Rieke, 1996)
Write:	<<[CRR96] N>>
N:	6
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	NGC 2024
Ref:	=1996ApJ...473..294C
by	COMERON F. , RIEKE G.H., RIEKE M.J.
	Astrophys. J., 473, 294-303 (1996)
	Properties of low-mass objects in NGC 2024.
o	Table 1: <[CRR96] N> (Nos 1-6)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRS2006]
[CRS2006]	(Cohen+Ryan+Straughn+, 2006)
Write:	<<[CRS2006] NNNNN>>
N:	45
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Photometric search for variable objects in the HUDF: 45 objects are selected in a catalog of 12514 objects.
in source:	NAME HUDF
Ref:	=2006ApJ...639..731C
by	COHEN S.H. , RYAN R.E.Jr, STRAUGHN A.N., HATHI N.P., WINDHORST R.A., KOEKEMOER A.M., PIRZKAL N., XU C., MOBASHER B., MALHOTRA S., STROLGER L.-G., RHOADS J.E.
	Astrophys. J., 639, 731-739 (2006)
	Clues to active galactic nucleus growth from optically variable objects in the Hubble Ultra Deep Field.
o	Table 2: <[CRS2006] NNNNN> N=45 among 12514.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRS2007]
[CRS2007]	(COntursi+Rubio+Sauvage+, 2007) (Not yet in Simbad)
Write:	<<[CRS2007] Star A>> <<[CRS2007] Knot N>> <<[CRS2007] Star N>>
N:	2+7
Object:	* + (IR) (SIMBAD class: Star)
Note:	ISOCAM-CVF observations of the HII region LHA 120-N 4.
in source:	Magellanic Clouds:LMC:LHA 120-N 4 = LHA 120-N 4
Ref:	=2007A&A...469..539C
by	CONTURSI A. , RUBIO M., SAUVAGE M., CESARSKY D., BARBA R., BOULANGER F.
	Astron. Astrophys., 469, 539-551 (2007)
	ISOCAM mid-infrared spectroscopy and NIR photometry of the HII complex N4 in the Large Magellanic Cloud.
o	Fig.1: <[CRS2007] Star A> (Nos A-B). Fig.3: <[CRS2007] Knot N> (Nos 1-2). Fig.5, Table 1: <[CRS2007] Star N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRS2011]
[CRS2011]	(Capak+Riechers+Scoville+, 2011)
Write:	<<[CRS2011] NNNNNNN>>
N:	10
Object:	G (SIMBAD class: Galaxy)
Note:	Spitzer IRAC observations of the COSMOS field.
Ref:	=2011Natur.470..233C
by	CAPAK P.L. , RIECHERS D., SCOVILLE N.Z., CARILLI C., COX P., NERI R., ROBERTSON B., SALVATO M., SCHINNERER E., YAN L., WILSON G.W., YUN M., CIVANO F., ELVIS M., KARIM A., MOBASHER B., STAGUHN J.G.
	Natur, 470, 233-235 (2011)
	A massive protocluster of galaxies at a redshift of z ~ 5.3.
o	Suppl. Table 1: <[CRS2011] NNNNNNN> N=10 among (Nos 1445777-1449472).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRS2013]
[CRS2013]	(Clarke+Randall+Sarazin+, 2013)
Write:	<<[CRS2013] N>>
N:	6
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS observations of N=6 compact X-ray sources in the field of ACO 2443.
in source:	ACO 2443
Ref:	=2013ApJ...772...84C
by	CLARKE T.E. , RANDALL S.W., SARAZIN C.L., BLANTON E.L., GIACINTUCCI S.
	Astrophys. J., 772, 84 (2013)
	Chandra view of the ultra-steep spectrum radio source in A2443: merger shock-induced compression of fossil radio plasma?
o	Paragr. 4.1: PCG 068859 is a misprint for PGC 068859.
o	Figs 1+3, Table 1: <[CRS2013] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRS93]
[CRS93]	(Caldwell+Rose+Sharples+, 1993)
Write:	<<[CRS93] NN>> <<[CRS93] WW NN>>
N:	133
Object:	G (SIMBAD class: Galaxy)
Note:	Table 1(a): central field, format 'NN', N=73 among N 97. Table 1(b): SW field, format 'SW NN', N=60 among 97.
in source:	ACO 1656 = Coma Cluster
Ref:	=1993AJ....106..473C
by	CALDWELL N. , ROSE J.A., SHARPLES R.M., ELLIS R.S., BOWER R.G.
	Astron. J., 106, 473-492 (1993)
	Star formation in early-type galaxies in the Coma cluster.
o	Table 1(a): <[CRS93] NN> central field, N=73 among 97. Table 1(b): <[CRS93] SW NN> SW field, N=60 among 97
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRS94]
[CRS94]	(Collura+Reale+Schulman+, 1994)
Write:	<<[CRS94] N>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
in source:	M 82 = NGC 3034
Ref:	=1994ApJ...420L..63C
by	COLLURA A. , REALE F., SCHULMAN E., BREGMAN J.N.
	Astrophys. J., 420, 63-66 (1994)
	Two very luminous variable X-ray sources in M 82.
o	Table 2: <[CRS94] N> N=2
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRS97]
[CRS97]	(Chini+Reipurth+Sievers+, 1997)
Write:	<<[CRS97] HH NN-NN MMS N>> <<[CRS97] HH NNN MMS>> <<[CRS97] IRAS 20050+2720 MMS N>>
N:	7+3+4+3
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
in source:	NAME HH 7-11
in source:	NAME HH 1-2
in source:	HH 114
in source:	HH 147
in source:	HH 108
in source:	HH 111
in source:	IRAS 20050+2720
Ref:	=1997A&A...325..542C
by	CHINI R. , REIPURTH B., SIEVERS A., WARD-THOMPSON D., HASLAM C.G.T., KREYSA E., LEMKE R.
	Astron. Astrophys., 325, 542-550 (1997)
	Cold dust around Herbig-Haro energy sources: morphology and new protostellar candidates.
o	p. 545: VLA 1, 2 = [RHR93] VLA 1, 2
o	<HH NNN> (Nos 165, 223). Table 1: <[CRS97] HH 7-11 MMS N> (Nos 1-3), <[CRS97] HH 1-2 MMS N> (Nos 1-3), <[CRS97] HH 114 MMS> N=1, <[CRS97] HH 147 MMS> N=1, <[CRS97] HH 108 MMS> N=1.
Ref:	=2001A&A...369..155C
by	CHINI R. , WARD-THOMPSON D., KIRK J.M., NIELBOCK M., REIPURTH B., SIEVERS A.
	Astron. Astrophys., 369, 155-169 (2001)
	Mm/Submm images of Herbig-Haro energy sources and candidate protostars.
o	Table 1: <[CRS97] HH 7-11 MMS N> (Nos 4-7) added, <[CRS97] HH 111 MMS> N=1, <[CRS97] IRAS 20050+2720 MMS N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CRSS
CRSS	(Cambridge ROSAT Serendipity Survey)
Write:	<<CRSS JHHMM.m+DDMM>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Only the first references from this survey are listed here. 1995MNRAS.272..462B: N=12 narrow em.-line X-ray galaxies. 1997MNRAS.285..511B: N=123 X-ray sources.
Ref:	=1995MNRAS.272..462B
by	BOYLE B.J. , McMAHON R.G., WILKES B.J., ELVIS M.
	Mon. Not. R. Astron. Soc., 272, 462-468 (1995)
	The Cambridge-Cambridge ROSAT serendipity survey - I. X-ray luminous galaxies.
o	Table 2: <CRSS JHHMM.m+DDMM> first ref. from this survey, N=12
Ref:	=1997MNRAS.285..511B
by	BOYLE B.J. , WILKES B.J., ELVIS M.
	Mon. Not. R. Astron. Soc., 285, 511-528 (1997)
	The Cambridge-Cambridge ROSAT Serendipity Survey - V. Catalogue and optical identifications.
o	Table 2: <CRSS JHHMM.m+DDMM> N=123, <[BWE97] JHHMMSS.s+DDMMSS> N=120.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CRT2007]
[CRT2007]	(Connelley+Reipurth+Tokunaga, 2007)
Write:	<<[CRT2007] IRAS 16288-2450(W)>>
N:	2
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	University of Hawaii 2.2m telescope observations. Use of archival 2MASS data.
in source:	IRAS 16288-2450
Ref:	=2007AJ....133.1528C
by	CONNELLEY M.S. , REIPURTH B., TOKUNAGA A.T.
	Astron. J., 133, 1528-1559 (2007)
	Infrared nebulae around young stellar objects.
o	Tables 1-2: <[CRT2007] IRAS 16288-2450(W)> (Nos IRAS 16288-2450(W), IRAS 16288-2450(E)).
=E=	Catalogue in electronic form as J/AJ/133/1528
Details on Acronym: [CRT2008]
[CRT2008]	(Connelley+Reipurth+Tokunaga, 2008)
Write:	<<[CRT2008] IRAS HHMMm+DDMM W>> <<[CRT2008] IRAS HHMMm+DDMM W NNa>>
N:	40+258
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Note:	NIR observations of Class I protostars with the UH 2.2m telescope, the NASA IRTF, UKIRT and Subaru.
Ref:	=2008AJ....135.2496C
by	CONNELLEY M.S. , REIPURTH B., TOKUNAGA A.T.
	Astron. J., 135, 2496-2525 (2008)
	The evolution of the multiplicity of embedded protostars. I. Sample properties and binary detections.
o	Table 1: <[CRT2008] IRAS HHMMm+DDMM W> N=40. Fig. 6: <[CRT2008] IRAS HHMMm+DDMM W NNa> N=258.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CRTS
CRTS	(Catalina Real-time Transient Survey)= (CSS) = (SSS) = (MLS)
Write:	<<CRTS {CSS\|SSS\|MLS}YYMMDD JHHMMSS+DDMMSS>> <<CRTS JHHMMSS.s+DDMMSS>> <<CRTS {CSS\|SSS\|MLS}YYMMDD:HHMMSS+DDMMSS>> (not recognised by Simbad, but found in literature)
N:	12+6+1+47055+42+27+855+1043
Object:	Poss. SN + Poss. CV + Bl? + V* (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	The Catalina Real-time Transient Survey (CRTS) reports the discovery of optical transients with three telescopes: Catalina Sky Survey 0.7m Schmidt (CSS), Siding Springs Survey 0.5m Schmidt (SSS) and Mt. Lemmon Survey 1.5m Cass (MLS). More info on the CRTS project can be found at http://crts.caltech.edu/ Updated lists of the transients discoveries are available at: http://nesssi.cacr.caltech.edu/catalina/Allns.html http://nesssi.cacr.caltech.edu/MLS/Allns.html http://nesssi.cacr.caltech.edu/SSS/Allns.html Format JHHMMSS.s+DDMMSS: introduced by Drake et al. (2014MNRAS.441.1186D) and Breedt et al. (2014MNRAS.443.3174B). In the latter publication, it is explained that "CRTS transients are assigned a detection ID in the form CSS\|SSS\|MLSYYMMDD JHHMMSS+DDMMSS [...]. Once the transient has been classified [...], it is assigned a CRTS identifier of the form CRTS JHHMMSS.s+DDMMSS." Only the first references are listed here. See also [DDM2009].
Ref:	=2008ATel.1734....1D
by	DRAKE A.J. , MAHABAL A.A., DJORGOVSKI S.G., WILLIAMS R., GRAHAM M.J., BESHORE E.C., LARSON S.M., HILL R., CATELAN M., CHRISTENSEN E.
	ATel, 1734, 1 (2008)
	Twelve CRTS Optical Transients.
o	<CRTS CSSYYMMDD JHHMMSS+DDMMSS> N=12.
Ref:	=2009ATel.2318....1D
by	DRAKE A.J. , DJORGOVSKI S.G., MAHABAL A.A., GRAHAM M.J., WILLIAMS R., CATELAN M., BESHORE E.C., LARSON S.M., BOATTINI A., GIBBS A., GRAUER A., HILL R., KOWALSKI R., CHRISTENSEN E.
	ATel, 2318, 1 (2009)
	The First Optical Transient Discoveries from MLS.
o	<CRTS MLSYYMMDD JHHMMSS+DDMMSS> N=6.
Ref:	=2010ATel.2620....1D
by	DRAKE A.J. , DJORGOVSKI S.G., MAHABAL A.A., GRAHAM M.J., WILLIAMS R., PRIETO J., CATELAN M., CHRISTENSEN E., McNAUGHT R., GARRADD G., BESHORE E.C., LARSON S.M.
	ATel, 2620, 1 (2010)
	A Supernova Candidate from the Siding Spring Survey.
o	<CRTS SSSYYMMDD JHHMMSS+DDMMSS> N=1.
Ref:	=2014ApJS..213....9D
by	DRAKE A.J. , GRAHAM M.J., DJORGOVSKI S.G., CATELAN M., MAHABAL A.A., TORREALBA G., GARCIA-ALVAREZ D., DONALEK C., PRIETO J.L., WILLIAMS R., LARSON S., CHRISTENSEN E., BELOKUROV V., KOPOSOV S.E., BESHORE E., BOATTINI A., GIBBS A., HILL R., KOWALSKI R., JOHNSON J., SHELLY F.
	Astrophys. J., Suppl. Ser., 213, 9 (2014)
	The Catalina surveys periodic variable star catalog.
o	Tables 3+8+9: <CRTS JHHMMSS.s+DDMMSS> N=47055+42+27.
Ref:	=2014MNRAS.441.1186D
by	DRAKE A.J. , GANSICKE B.T., DJORGOVSKI S.G., WILS P., MAHABAL A.A., GRAHAM M.J., YANG T.-C., WILLIAMS R., CATELAN M., PRIETO J.L., DONALEK C., LARSON S., CHRISTENSEN E.
	Mon. Not. R. Astron. Soc., 441, 1186-1200 (2014)
	Cataclysmic variables from the Catalina Real-time Transient Survey.
o	Table 1: <CRTS JHHMMSS.s+DDMMSS> N=855.
Ref:	=2014MNRAS.443.3174B
by	BREEDT E. , GANSICKE B.T., DRAKE A.J., RODRIGUEZ-GIL P., PARSONS S.G., MARSH T.R., SZKODY P., SCHREIBER M.R., DJORGOVSKI S.G.
	Mon. Not. R. Astron. Soc., 443, 3174-3207 (2014)
	1000 cataclysmic variables from the Catalina Real-time Transient Survey.
o	<CRTS JHHMMSS.s+DDMMSS> N=1043.
=E=	Catalogue in electronic form as J/ApJS/213/9
=E=	Catalogue in electronic form as J/MNRAS/441/1186
=E=	Catalogue in electronic form as <J/MNRAS/443/3174/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Cru
Cru	(Crux)
*****	Avoid the usage of Cru, prefer [ABC89]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cru
Cru	(Crux Assoc.)
*****	Avoid the usage of Cru, prefer Glazar
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cru
Cru	(Crux)
*****	Avoid the usage of Cru, prefer [MWC53]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Cru
Cru	(Crux)
*****	Avoid the usage of Cru, prefer [PF96]
Origin	of the Acronym: A (1997AJ....113.2130F)
Details on Acronym: CRVAD
CRVAD	(Catalogue of Radial Velocities with Astrometric Data) (Not yet in Simbad)
Write:	<<CRVAD HH.hhhhhhhhh+DD.dddddddd>>
N:	34553
Object:	* (SIMBAD class: Star)
Note:	Catalogue of radial velocities of stars with high precision astrometric data, from the ASCC-2.5 catalogue.
Ref:	=2004AN....325..439K
by	KHARCHENKO N.V. , PISKUNOV A.E., SCHOLZ R.-D.
	Astron. Nachr., 325, 439-444 (2004)
	The catalogue of radial velocities of galactic stars with high precision astrometric data (CRVAD).
o	Catalogue: <CRVAD HH.hhhhhhhhh+DD.dddddddd> N=34553.
=E=	Catalogue in electronic form as III/239
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CRW
CRW	(Chini+Reipurth+Ward-Thompson+)
*****	Avoid the usage of CRW, prefer [CRW97]
Origin	of the Acronym: L (2002A&A...392..239S)
Details on Acronym: [CRW2013]
[CRW2013]	(Carilli+Riechers+Walter+, 2013)
Write:	<<[CRW2013] SMG>> <<[CRW2013] Lyalpha-N>>
N:	1+2 (SIMBAD class: Galaxy)
Note:	ALMA 340GHz CII line observations of the field of a Submillimeter Galaxy.
Ref:	=2013ApJ...763..120C
by	CARILLI C.L. , RIECHERS D., WALTER F., MAIOLINO R., WAGG J., LENTATI L., McMAHON R., WOLFE A.
	Astrophys. J., 763, 120 (2013)
	The anatomy of an extreme starburst within 1.3 gyr of the big bang revealed by ALMA.
o	Table 1: <[CRW2013] SMG> N=1, <[CRW2013] Lyα-N> (Nos 1-2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CRW97]
[CRW97]	(Chini+Reipurth+Ward-Thompson+, 1997)= (CRW) = (MMS)
Write:	<<[CRW97] OMC-3 MMS NN>>
N:	10
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
in source:	OMC:OMC 3 = OMC 3
Ref:	=1997ApJ...474L.135C
by	CHINI R. , REIPURTH B., WARD-THOMPSON D., BALLY J., NYMAN L.-A., SIEVERS A., BILLAWALA Y.
	Astrophys. J., 474, 135-138 (1997)
	Dust filaments and star formation in OMC-2 and OMC-3.
o	Table 1: <[CRW97] OMC-3 MMS NN> (Nos 1-10). Table 1: <[MWZ90] OMC-2 FIR Na> (Nos 1a-1c, 6a-6d)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CRX
CRX	(Crampton, X source)
*****	Avoid the usage of CRX, prefer C84
Origin	of the Acronym: L (1993A&A...272...77B)
Details on Acronym: cs
cs	(Century Survey)
*****	Avoid the usage of cs, prefer [BGF2001]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CS
CS	(Curtis Schmidt telescope)
*****	Avoid the usage of CS, prefer BPS
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CS
CS	(Carbon Star)
*****	Avoid the usage of CS, prefer CGCS
Origin	of the Acronym: L (2000IBVS.4842....1Y)
Details on Acronym: CS
CS	(Comeron+Schneider)
*****	Avoid the usage of CS, prefer [CS2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CS
CS	(Christian+Schommer)
*****	Avoid the usage of CS, prefer [CS82]
Origin	of the Acronym: L (1999ApJS..122..431C)
Details on Acronym: CS
CS	(Clowes+Savage)
*****	Avoid the usage of CS, prefer [CS83]
Origin	of the Acronym: L (1991AJ....102..502G)
Details on Acronym: CS
CS	(CS observation)
*****	Avoid the usage of CS, prefer [KSH92]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CS
CS	(Continuum Source)
*****	Avoid the usage of CS, prefer [MSB86]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CS
CS	(Coalsack)
*****	Avoid the usage of CS, prefer [RWW88]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CS
CS	(Compact Source)
*****	Avoid the usage of CS, prefer [SGZ91]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CS
CS	(Continuum Source)
*****	Avoid the usage of CS, prefer [YMK91]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CS1
CS1	(Caldwell+Schechter, 1st catalog)
*****	Avoid the usage of CS1, prefer [CS96]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CS2
CS2	(Caldwell+Schechter, 2st catalog)
*****	Avoid the usage of CS2, prefer [CS96]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CS2000]
[CS2000]	(Canalizo+Stockton, 2000)
Write:	<<[CS2000] N>>
N:	9
Object:	? (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck LRIS observations. N=9 serendipitous objects around 3C 48.
Ref:	=2000ApJ...528..201C
by	CANALIZO G. , STOCKTON A.
	Astrophys. J., 528, 201-218 (2000)
	3C 48: stellar populations and the kinematics of stars and gas in the host galaxy.
o	p. 209 : G 515 = [HO93] 7-515, p. 216 : IR 0759+651 = QSO 0759+651
o	Table 3: <[CS2000] N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CS2001]
[CS2001]	(Canalizo+Stockton, 2001)
Write:	<<[CS2001] companion galaxy>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck II LRIS spectroscopic and UH 2.2m telescope imaging observations of IRAS 04505-2958.
Ref:	=2001ApJ...555..719C
by	CANALIZO G. , STOCKTON A.
	Astrophys. J., 555, 719-743 (2001)
	Quasi-stellar objects, ultraluminous infrared galaxies, and mergers.
o	Paragr. 3.3: <[CS2001] companion galaxy> N=1.
o	Fig. 4 and Fig. 8 : Stars not in SIMBAD
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CS2003]
[CS2003]	(Codella+Scappini, 2003)
Write:	<<[CS2003] Blue N>> <<[CS2003] Red N>>
N:	2+3
Object:	CO peak (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	IRAM 30m telescope observations. N=3 molecular clumps in [CB88] 34. See also [CSB2002b].
in source:	[CB88] 34
Ref:	=2003MNRAS.344.1257C
by	CODELLA C. , SCAPPINI F.
	Mon. Not. R. Astron. Soc., 344, 1257-1263 (2003)
	The young cluster in the CB34 globule: the clumps and the outflows.
o	Submillimetre sources e.g. in Fig. 1 are [HSW99] CB 34 SMM N in SIMBAD.
o	Fig.5: <[CS2003] Blue N> (Nos 1-2), <[CS2003] Red N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CS2004]
[CS2004]	(Connolly+SDSS Collaboration, 2004)= [CS2004a]
Write:	<<[CS2004] JHHMMSS.ss+DDMMSS.s>>
N:	7
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	SDSS observations. Host galaxies of SN 2004CJ to SN 2004CP.
Ref:	=2004IAUC.8359....1C
by	CONNOLLY A. , (The SDSS Collaboration)
	IAU Circ., 8359, 1-None (2004)
	Supernovae 2004cj-2004cq.
o	<[CS2004] JHHMMSS.ss+DDMMSS.s> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CS2004a]
[CS2004a]	(Connolly+SDSS Collaboration, 2004)
*****	Avoid the usage of [CS2004a], prefer [CS2004]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CS2004b]
[CS2004b]	(Cannon+Skillman, 2004)
Write:	<<[CS2004b] A>>
N:	4
Object:	(Rad) (SIMBAD class: cmRad = Centimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA multifrequency imaging of NGC 625. N=4 radio continuum emission sources are observed. [CDS2003] NGC 625 A, B, C are the optical counterparts of [CS2004b] A, B, C, but not D.
in source:	NGC 625
Ref:	=2004ApJ...610..772C
by	CANNON J.M. , SKILLMAN E.D.
	Astrophys. J., 610, 772-780 (2004)
	The nature of radio continuum emission in the dwarf starburst galaxy NGC 625.
o	Table 3: <[CS2004b] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CS2006]
[CS2006]	(CHristopher+Smail, 2006)
Write:	<<[CS2006] FSNNN-NN>>
N:	111
Object:	G (SIMBAD class: Galaxy)
Note:	Catalogue of faint galaxies situated close to standard FS stars. Use of UKIRT archival data. See also FSAO designations of these objects.
Ref:	=2006MNRAS.365..439C
by	CHRISTOPHER N.M. , SMAIL I.
	Mon. Not. R. Astron. Soc., 365, 439-446 (2006)
	A catalogue of potential adaptive optics survey fields from the UKIRT archive.
o	Table 2, col(1): <[CS2006] FSNNN-NN> N=111 = Table 2, col(2): <FSAO JHHMMSS.ss+DDMMSS.s> N=111.
=E=	Catalogue in electronic form as J/MNRAS/365/439
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CS2007]
[CS2007]	(Comeron+Schneider, 2007)= (CS)
Write:	<<[CS2007] NNN>>
N:	147
Object:	* (SIMBAD class: Star)
Note:	VLT NACO images of RCW 108. New stars, not listed in 2005A&A...433..955C, see also [CSR2005].
in source:	RCW 108
Ref:	=2007A&A...473..149C
by	COMERON F. , SCHNEIDER N.
	Astron. Astrophys., 473, 149-162 (2007)
	A close look at the heart of RCW 108.
o	Table 2: <[CS2007] NNN> (Nos 1-147). Table 2: <[CSR2005] Star NNA> N=18.
=E=	Catalogue in electronic form as J/A+A/473/149
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CS2009]
[CS2009]	(Corbally+Straizys, 2009)= ([CS2009a])
Write:	<<[CS2009] Gahm NN>>
N:	4
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Note:	Steward Observatory 2.3m telescope spectroscopy of young stars in the Camelopardalis and Perseus dark clouds.
Ref:	=2009BaltA..18....1C
by	CORBALLY C.J. , STRAIZYS V.
	BaltA, 18, 1-18 (2009)
	Young stars in the Camelopardalis dust and molecular clouds. V. More YSOs confirmed spectroscopically.
o	Tables 1-2: <[CS2009] Gahm NN> (Nos 2, 4, 11, 24).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CS2011]
[CS2011]	(Carraro+Seleznev, 2011)
Write:	<<[CS2011] NNNN>>
N:	41+28
Object:	Poss. Blue Straggler * + Poss. HB* (SIMBAD class: Star)
Note:	ESO NTT EFOSC2 observations of N=41 blue straggler star candidates and N=28 HB star candidates.
in source:	Cl Arp 2
Ref:	=2011MNRAS.412.1361C
by	CARRARO G. , SELEZNEV A.F.
	Mon. Not. R. Astron. Soc., 412, 1361-1366 (2011)
	An analysis of the blue straggler population in the Sgr dSph globular cluster Arp 2.
o	Tables 1-2: <[CS2011] NNNN> N=41+28 among (Nos 125-6087).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CS2018]
[CS2018]	(Costa+Spangler, 2018)
Write:	<<[CS2018] W4-ANN>>
N:	36
Object:	(Radio) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 4.3GHz and 7.76Hz continuum observations of N=32 radio sources whose lines of sight pass through or near to the shell of the IC 1805 stellar bubble. See also [SSF2013].
in source:	NAME Heart Nebula
Ref:	=2018ApJ...865...65C
by	COSTA A.H. , SPANGLER S.R.
	Astrophys. J., 865, 65-65 (2018)
	A Faraday rotation study of the stellar bubble and H II region associated with the W4 complex.
o	Table 1: <[CS2018] W4-ANN> N=24+8 among (Nos I1-I24, O1-O10). Table 5: <[CS2018] W4-ONN> (Nos O3, O19, O26-O27) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CS62]
[CS62]	(Cousins+Stoy, 1962)= (E)
Write:	<<[CS62] EN NNN>> <<[CS62] EN A>> <<[CS62] EN a>>
N:	1140
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Study of stars in the E1 to E9 regions. Formats 'EN NNN' N=801, 'EN A' N=55, and 'EN a' N=90 The format 'ENNNN' is also used instead of 'EN NNN' in literature.
in source:	NAME E1 Region
in source:	NAME E2 Region
in source:	NAME E3 Region
in source:	NAME E4 Region
in source:	NAME E5 Region
in source:	NAME E6 Region
in source:	NAME E7 Region
in source:	NAME E8 Region
in source:	NAME E9 Region
Ref:	=1962RGOB...49....3C
by	COUSINS A.W.J. , STOY R.H.
	R. Obs. Bull., 49, 3-None (1962)
	Standard magnitudes in the E regions.
o	<[CS62] EN NNN> N=801, <[CS62] EN A> N=3, <[CS62] EN a> N=60. <NAME E1 REGION> to <NAME E9 REGION> N=9
Ref:	=1982PASP...94..244G
by	GRAHAM J.A.
	Publ. Astron. Soc. Pac., 94, 244-265 (1982)
	UBVRI standard stars in the E-regions.
o	object I(tableIII) not [CS62] E2 I
o	Tables II-X: <[CS62] EN A> N=52 are new, <[CS62] EN a> N=30 are new
=E=	Catalogue in electronic form as II/222
=E=	Catalogue in electronic form as <J/PASP/94/244/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CS82]
[CS82]	(Christian+Schommer, 1982)= (CS)
Write:	<<[CS82] N>> <<[CS82] ANNNa>>
Object:	Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Format 'N' (Nos 1-9), is used for obj. not on plate 8. In the format 'ANNN' the letter 'A' stands for: 'CNN' for Cluster, N=39. 'HNN' for HII, N=49. 'UNNNa' for Unclassified, N=160. 'MNN' for Miscellaneous, N=18. 'ON' ?, N=2, meaning not identified. 'RNN' for obj. from Racine, unpublished. 'SNNNa' for obj. from Sandage, unpublished.
in source:	M 33 = NGC 598
Ref:	=1982ApJS...49..405C
by	CHRISTIAN C.A. , SCHOMMER R.A.
	Astrophys. J., Suppl. Ser., 49, 405-424 (1982)
	The cluster system of M 33.
o	<[CS82] CNN> (Nos C1-C39), <[CS82] HNN> (Nos H1-H49), <[CS82] UNNN> (Nos U1-U160), <[CS82] MNN> (Nos M1-M18), <[CS82] N> (Nos 1-9).
Ref:	=1988AJ.....95..704C
by	CHRISTIAN C.A. , SCHOMMER R.A.
	Astron. J., 95, 704-719 (1988)
	BVI photometry of star clusters in M 33.
o	Table III: <[CS82] ON> (Nos O1-O3), <[CS82] RNN> (Nos R12-R15), <[CS82] SNNNa> N=21 among (Nos S24-S248), <[CS82] UNNa> (No. 84a) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CS83]
[CS83]	(Clowes+Savage, 1983)= (CS) = ([CS83a])
Write:	<<[CS83] HHMM+DDd>> <<[CS83] HHMM+DDMM>> <<[CS83] NNN>>
N:	210
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Ref:	=1983MNRAS.204..365C
by	CLOWES R.G. , SAVAGE A.
	Mon. Not. R. Astron. Soc., 204, 365-375 (1983)
	Optically-selected quasar candidates in a field containing South Galactic Pole.
o	<[CS83] HHMM+DDd> or <[CS83] HHMM+DDdd>, <[CS83] NNN> N=210
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CS83a]
[CS83a]	(Clowes+Savage, 1983)
*****	Avoid the usage of [CS83a], prefer [CS83]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CS83b]
[CS83b]	(Cohen+Schwartz, 1983)= (IRS)
Write:	<<[CS83b] NGC NNNN IRS N>> <<[CS83b] HH NN IRS N>> <<[CS83b] RNO NN IRS N>> <<[CS83b] HH NN-NN-NN IRS N>>
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Infrared sources in the vicinity of HH objects: NGC 1333, 2264, 7129, HH 31, 32, 33-40-34, 43, RNO 40, 43
Ref:	=1983ApJ...265..877C
by	COHEN M. , SCHWARTZ R.D.
	Astrophys. J., 265, 877-900 (1983)
	The exciting stars of Herbig-Haro objects.
o	VLA associated with SSV LDN 1551 5 = [CBS82] 042840.226+180142.00
o	Tables 1, 2, 3: <[CS83b] NGC 1333 IRS N> (Nos 1-2), <[CS83b] NGC 2264 IRS N> (Nos 1-3), <[CS83b] NGC 7129 IRS N> (Nos 1-4), <[CS83b] HH 31 IRS N> (Nos 1-4), <[CS83b] HH 43 IRS N> (Nos 1-2), <[CS83b] HH 32 IRS N> (Nos 1-4), <[CS83b] HH 33-40-34 IRS N> (Nos 1-9), <[CS83b] RNO 40 IRS N> (Nos 1-3), <[CS83b] RNO 43 IRS N> (Nos 1-2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CS86]
[CS86]	(Carney+Seitzer, 1986)
Write:	<<[CS86] N-NNNN>>
N:	1671
Object:	* (SIMBAD class: Star)
Note:	Kitt Peak observations. CCD photometry of 2 fields (1 and 2) in the Draco Dwarf Galaxy.
in source:	NAME Draco Dwarf Galaxy
Ref:	=1986AJ.....92...23C
by	CARNEY B.W. , SEITZER P.
	Astron. J., 92, 23-42 (1986)
	Deep photometry of the Draco dwarf spheroidal galaxy.
o	Table I(a): <[CS86] 1-NNNN> (Nos 1-1 to 1-1039). Table I(b): <[CS86] 2-NNN> (Nos 2-1 to 2-875).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CS87]
[CS87]	(Couch+Sharples, 1987)
Write:	<<[CS87] AC103 NNN>> <<[CS87] AC114 NNN>> <<[CS87] AC118 NNN>>
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	See also 1985MNRAS.212..687S See also CN
in source:	ACCG 103 = ACO S 910
in source:	ACCG 114 = ACO S 1077
in source:	ACCG 118 = ACO 2744
Ref:	=1987MNRAS.229..423C
by	COUCH W.J. , SHARPLES R.M.
	Mon. Not. R. Astron. Soc., 229, 423-456 (1987)
	A spectroscopic study of three rich galaxy clusters at ζ=0.31.
o	Table 2: <[CS87] AC103 NNN> = <CN AC103 NNN> N=60 among 430. Table 3: <[CS87] AC114 NNN> = <CN AC114 NNN> N=52 among 859. Table 4: <[CS87] AC118 NNN> = <CN AC118 NNN> N=40 among 398.
Ref:	=1994ApJ...430..121C
by	COUCH W.J. , ELLIS R.S., SHARPLES R.M., SMAIL I.
	Astrophys. J., 430, 121-138 (1994)
	Morphological studies of the galaxy populations in distant "Butcher-Oemler" clusters with HST. I. AC 114 at z = 0.31 and Abell 370 at z = 0.37.
o	Tables 2, 3, 4: <[CS87] AC114 NNN> = <CN AC114 NNN> Nos among (Nos 30-832).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CS92]
[CS92]	(Cernis+Straizys, 1992)
Write:	<<[CS92] NN>>
N:	14
Object:	* (SIMBAD class: Star)
Ref:	=1992BaltA...1..163C
by	CERNIS K. , STRAIZYS V.
	Baltic Astronomy, 1, 163-167 (1992)
	On the distance of the high latitude dark cloud Lynds 134 in Serpens.
o	<[CS92] NN> N=14
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CS96]
[CS96]	(Caldwell+Schechter, 1996)= (CS1) = (CS2)
Write:	<<[CS96] 1-NNNNN>> <<[CS96] 2-NNNNN>>
N:	29877+18811
Object:	* (SIMBAD class: Star)
Note:	* in 2 regions near the SGP, region 1: sidereal, region 2 double sidereal mode.
Ref:	=1996AJ....112..772C
by	CALDWELL J.A.R. , SCHECHTER P.L.
	Astron. J., 112, 772-780 (1996)
	Scanned CCD V and I photometry at the South Galactic Pole.
o	(Erratum) + Erratum: 1996 AJ 112, p. 1730
o	<[CS96] 1-NNNNN> N=29877, <[CS96] 2-NNNNN> N=18811
=E=	Catalogue in electronic form as J/AJ/112/772
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSA2000]
[CSA2000]	(Capetti+Schreier+Axon+, 2000) (Not yet in Simbad)
Write:	<<[CSA2000] SN>>
N:	2
Object:	Feature (SIMBAD class: Infrared = Infra-Red Source)
Note:	HST NICMOS observations of Cen A. N=2 elongated features body of the S-shaped structure.
in source:	Cen A = NGC 5128
Ref:	=2000ApJ...544..269C
by	CAPETTI A. , SCHREIER E.J., AXON D., YOUNG S., HOUGH J.H., CLARK S., MARCONI A., MACCHETTO D., PACKHAM C.
	Astrophys. J., 544, 269-276 (2000)
	Hubble space telescope infrared imaging polarimetry of Centaurus A: implications for the unified scheme and the existence of a misdirected BL Lacertae nucleus.
o	Fig.2: <[CSA2000] SN> (Nos S1-S2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSA2014]
[CSA2014]	(Calamida+Sahu+Anderson+, 2014) (Not yet in Simbad)
Write:	<<[CSA2014] NN>>
N:	74
Object:	Poss. WD (SIMBAD class: Star)
Note:	HST ACS observations of N=74 candidate bulge white dwarfs (DWs).
in source:	NAME Galactic Bulge
Ref:	=2014ApJ...790..164C
by	CALAMIDA A. , SAHU K.C., ANDERSON J., CASERTANO S., CASSISI S., SALARIS M., BROWN T., SOKOL J., BOND H.E., FERRARO I., FERGUSON H., LIVIO M., VALENTI J., BUONANNO R., CLARKSON W., PIETRINFERNI A.
	Astrophys. J., 790, 164 (2014)
	First detection of the white dwarf cooling sequence of the Galactic bulge.
o	Table 1: <[CSA2014] NN> (Nos 1-74).
=E=	Catalogue in electronic form as <J/ApJ/790/164/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSA2018]
[CSA2018]	(Cerny+Sharon+Andrade-Santos+, 2018)
Write:	<<[CSA2018] Abell NNNN N>> <<[CSA2018] Abell NNNN NN.N>> <<[CSA2018] RXC JHHMM.m+DDMM N>> <<[CSA2018] RXC JHHMM.m+DDMM N.N>> <<[CSA2018] ACT-CL J0102-49151 NN>> <<[CSA2018] ACT-CL J0102-49151 NN.N>>
N:	8+7+11+37+25+30
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	N=37+25+30 gravitationally lensed images in N=8+7+11 multiply-imaged background sources, by five galaxy clusters (Abell 2537, Abell 2163, RXC J0142.9+4438, RXC J2211.7–0349, and ACT-CLJ0102–49151). Use of data from the RELICS Hubble Treasury program. See also [AAZ2019], [ACZ2018], [CAZ2018], [PSC2018].
in source:	ACO 2537
in source:	ACO 2163
in source:	RXC J0142.9+4438
in source:	RXC J2211.7-0350
in source:	ACT-CL J0102-4915
Ref:	=2018ApJ...859..159C
by	CERNY C. , SHARON K., ANDRADE-SANTOS F., AVILA R.J., BRADAC M., BRADLEY L.D., CARRASCO D., COE D., CZAKON N.G., DAWSON W.A., FRYE B.L., HOAG A., HUANG K.-H., JOHNSON T.L., JONES C., LAM D., LOVISARI L., MAINALI R., OESCH P.A., OGAZ S., PAST M., PATERNO-MAHLER R., PETERSON A., RIESS A.G., RODNEY S.A., RYAN R.E., SALMON B., SENDRA-SERVER I., STARK D.P., STROLGER L.-G., TRENTI M., UMETSU K., VULCANI B., ZITRIN A.
	Astrophys. J., 859, 159-159 (2018)
	RELICS: strong lens models for five galaxy clusters from the Reionization Lensing Cluster Survey.
o	Figs 1+5, Tables 5+13: <[CSA2018] Abell NNNN N> N=4+4, <[CSA2018] Abell NNNN NN.N> N=25+12. Figs 2+3, Tables 7+9: <[CSA2018] RXC JHHMM.m+DDMM N> N=4+3, <[CSA2018] RXC JHHMM.m+DDMM N.N> N=14+11. Fig. 4, Table 11: <[CSA2018] ACT-CL J0102-49151 NN> N=11, <[CSA2018] ACT-CL J0102-49151 NN.N> N=30.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSB2000]
[CSB2000]	(Canalizo+Stockton+Brotherton+, 2000)
Write:	<<[CSB2000] UN J1025-0040 C>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Note:	N=1 companion galaxy ('C') of UN J1025-0040. This S-SW companion is already seen in Fig.2 of Paper I: 1999ApJ...520L..87B.
Ref:	=2000AJ....119...59C
by	CANALIZO G. , STOCKTON A., BROTHERTON M.S., VAN BREUGEL W.
	Astron. J., 119, 59-62 (2000)
	A companion galaxy to the poststarburst quasar UN J1025-0040.
o	The companion galaxy, without designation given by authors, is named '[CSB2000] UN J1025-0040 C' in SIMBAD.
o	Fig.2: <[CSB2000] UN J1025-0040 C> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSB2002]
[CSB2002]	(Chapman+Scott+Borys+, 2002)
Write:	<<[CSB2002] Cl 0016+16 A>> <<[CSB2002] MS HHMM+DD A>> <<[CSB2002] ACO NNNN A>> <<[CSB2002] ZwCl 3146 A>> <<[CSB2002] SMM JHHMMm+DDMM>> <<[CSB2002] SMM JHHMMm+DDMMm>>
N:	17
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	N=17 submm sources in 8 ClG.
in source:	ClG 0016+1609 = 1E 0015.9+1609
in source:	1E 0451.6-0305 = ClG 0451-0305
in source:	ACO 520 = 1E 0451.5+0250
in source:	ZwCl 3146
in source:	ClG 1054-0321 = 1E 1054.4-0321
in source:	ClG 1455+2232 = 1E 1455.0+2232
in source:	ACO 2219
in source:	ACO 2261
Ref:	=2002MNRAS.330...92C
by	CHAPMAN S.C. , SCOTT D., BORYS C., FAHLMAN G.G.
	Mon. Not. R. Astron. Soc., 330, 92-104 (2002)
	Submillimetre sources in rich cluster fields: source counts, redshift estimates and cooling flow limits.
o	<[CSB2002] Cl 0016+16 A>, <[CSB2002] MS HHMM+DD A>, <[CSB2002] ACO NNNN A>, <[CSB2002] ZwCl 3146 A>, N=17 = <[CSB2002] SMM JHHMMm+DDMM>, <[CSB2002] SMM JHHMMm+DDMMm>, N=17.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSB2002a]
[CSB2002a]	(Chapman+Scott+Borys+, 2002)
*****	Avoid the usage of [CSB2002a], prefer [CSB2002]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSB2002b]
[CSB2002b]	(Codella+Scappini+Bachiller+, 2002)
Write:	<<[CSB2002b] A>>
N:	3
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=2 blueshifted clumps and N=3 redshifted clumps in the CO map of [CB88] 34. See also [CS2003].
in source:	[CB88] 34
Ref:	=2002MNRAS.331..893C
by	CODELLA C. , SCAPPINI F., BACHILLER R., BENEDETTINI M.
	Mon. Not. R. Astron. Soc., 331, 893-900 (2002)
	SO and SiO emission around the young cluster in the CB34 globule.
o	Submillimetre sources e.g. in Figs are [HSW99] CB 34 SMM N in SIMBAD.
o	Fig.2: <[CSB2002b] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSB2004]
[CSB2004]	(Croom+Schade+Boyle+, 2004)= ([CSB2004a])
Write:	<<[CSB2004] JHHMMSS.ss+DDMMSS.s>>
N:	9
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	PSF (Point-Spread Function) calibration stars for Gemini North AO observations (AO=Adaptive Optics).
Ref:	=2004ApJ...606..126C
by	CROOM S.M. , SCHADE D., BOYLE B.J., SHANKS T., MILLER L., SMITH R.J.
	Astrophys. J., 606, 126-138 (2004)
	Gemini imaging of QSO host galaxies at z~2.
o	Table 2, col(2, 3): <[CSB2004] JHHMMSS.ss+DDMMSS.s> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSB2004a]
[CSB2004a]	(Croom+Schade+Boyle+, 2004)
*****	Avoid the usage of [CSB2004a], prefer [CSB2004]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSB2004b]
[CSB2004b]	(Chapman+Smail+Blain+, 2004)
Write:	<<[CSB2004b] RG JHHMMSS.ss+DDMMSS.s>>
N:	18
Object:	rG (SIMBAD class: RadioG = Radio Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck spectroscopic redshifts for 18 sub-mm quiet Optically Faint Radio Galaxies (OFRG).
Ref:	=2004ApJ...614..671C
by	CHAPMAN S.C. , SMAIL I., BLAIN A.W., IVISON R.J.
	Astrophys. J., 614, 671-678 (2004)
	A population of hot, dusty ultraluminous galaxies at z~2.
o	Table 1: <[CSB2004b] RG JHHMMSS.ss+DDMMSS.s> N=18.
=E=	Catalogue in electronic form as J/ApJ/614/671
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSB2005]
[CSB2005]	(Cotter+Simpson+Bolton, 2005)= ([CSB2005a]) = (TH)
Write:	<<[CSB2005] NN>>
N:	18
Object:	Extremely Red Obj. (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	NIR spectroscopy of ERO objects using the OHS/CISCO spectrograph at the Subaru telescope. The 18 objects are designated 'TH NN' by the authors, they are from T. Haynes Thesis (1998).
Ref:	=2005MNRAS.360..685C
by	COTTER G. , SIMPSON C., BOLTON R.C.
	Mon. Not. R. Astron. Soc., 360, 685-692 (2005)
	Vigorous star formation in a bulge-dominated extremely red object at z= 1.34.
o	Table 1: <[CSB2005] NN> (Nos 1-18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSB2005a]
[CSB2005a]	(Cotter+Simpson+Bolton, 2005)
*****	Avoid the usage of [CSB2005a], prefer [CSB2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSB2005b]
[CSB2005b]	(Cenko+Soifer+Bian+, 2005)
Write:	<<[CSB2005b] SN>>
N:	7
Object:	? (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Keck LRIS and VLT observations of GRB 050509b: N=7 sources are found in the field.
Ref:	=2005GCN..3401....1C
by	CENKO S.B. , SOIFER B.T., BIAN C., DESAI V., KULKARNI S.R., BERGER E., DEY A., JANNUZI B.T.
	GRB Coordinates Network, Circular Service, 3401, 1-None (2005)
	GRB 050509b: further analysis of Keck LRIS images.
o	<[CSB2005b] SN> (Nos S1-S4).
Ref:	=2005GCN..3410....1H
by	HJORTH J. , SOLLERMAN J., JENSEN B.L., FYNBO J.P.U., JAKOBSSON P., CASTRO CERON J.M., PEDERSEN K., PEDERSEN H., WATSON D., STARLING R., GOROSABEL J., RAMIREZ-RUIZ E., KOUVELIOTOU C.
	GRB Coordinates Network, Circular Service, 3410, 1-None (2005)
	GRB050509B: optical observations at the very large telescope.
o	<[CSB2005b] SN> (Nos S5-S6) added.
Ref:	=2005GCN..3422....1K
by	KOSUGI G. , FURUSAWA H., TAKADA M., KAWAI N.
	GRB Coordinates Network, Circular Service, 3422, 1-None (2005)
	GRB 050509B: Subaru optical observations.
o	<[CSB2005b] SN> (No. S7) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSB2008]
[CSB2008]	(Chomiuk+Strader+Brodie+, 2008)
Write:	<<[CSB2008] UVN>> <<[CSB2008] LN>> <<[CSB2008] GCNN>>
N:	6+1+13
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Stat:	is completely incorporated in Simbad
Note:	HST photometry and Keck spectroscopy of globular clusters in NGC 7457.
in source:	NGC 7457
Ref:	=2008AJ....136..234C
by	CHOMIUK L. , STRADER J., BRODIE J.P.
	Astron. J., 136, 234-249 (2008)
	The peculiar globular cluster system of the S0 galaxy NGC 7457.
o	Table 2: <[CSB2008] UVN> (Nos UV1-UV6), <[CSB2008] LN> (No. L1). Table 3: <[CSB2008] GCNN> (Nos GC1-GC13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSB2011]
[CSB2011]	(Cain+Schechter+Bautz, 2011) (Not yet in Simbad)
Write:	<<[CSB2011] NN>>
N:	50
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=50 objects with the largest 1-flexion S/N in the field of ACO 1689. Use of Hubble Legacy Archive data.
in source:	ACO 1689
Ref:	=2011ApJ...736...43C
by	CAIN B. , SCHECHTER P.L., BAUTZ M.W.
	Astrophys. J., 736, 43 (2011)
	Measuring gravitational lensing flexion in A1689 using an Analytic Image Model.
o	Table 2: <[CSB2011] NN> (Nos 1-50).
=E=	Catalogue in electronic form as <J/ApJ/736/43/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSB2012]
[CSB2012]	(Capozzi+Spavone+Barbati+, 2012)
Write:	<<[CSB2012] SHK NNN NN>>
N:	105
Object:	G (SIMBAD class: Galaxy)
Note:	TNG DOLORES observations of N=105 galaxies in five Shakhbazian groups of galaxies. Use of SDSS data.
in source:	Shk 10
in source:	Shk 71
in source:	Shk 75
in source:	Shk 80
in source:	Shk 259
Ref:	=2012MNRAS.426.2019C
by	CAPOZZI D. , SPAVONE M., BARBATI S., PAOLILLO M., DE FILIPPIS E., LONGO G.
	Mon. Not. R. Astron. Soc., 426, 2019-2045 (2012)
	Characterizing galaxy groups: spectroscopic observations of the Shakhbazyan sample.
o	Tables A1-A5: <[CSB2012] SHK NNN NN> N=25+21+19+21+19.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSB2017]
[CSB2017]	(Cesaroni+Sanchez-Monge+Beltran+, 2017) (Not yet in Simbad)
Write:	<<[CSB2017] {G345.50M\|G345.50S}>>
N:	2
Object:	Molecular core (SIMBAD class: denseCore = Dense Core)
Note:	Detection of N=2 molecular cores in G345.50 using ALMA band 6 0.”2 resolution data.
in source:	IRAS 17008-4040
Ref:	=2017A&A...602A..59C
by	CESARONI R. , SANCHEZ-MONGE A., BELTRAN M.T., JOHNSTON K.G., MAUD L.T., MOSCADELLI L., MOTTRAM J.C., AHMADI A., ALLEN V., BEUTHER H., CSENGERI T., ETOKA S., FULLER G.A., GALLI D., GALVAN-MADRID R., GODDI C., HENNING T., HOARE M.G., KLAASSEN P.D., KUIPER R., KUMAR M.S.N., LUMSDEN S., PETERS T., RIVILLA V.M., SCHILKE P., TESTI L., VAN DER TAK F., VIG S., WALMSLEY C.M., ZINNECKER H.
	Astron. Astrophys., 602A, 59-59 (2017)
	Chasing discs around O-type (proto)stars: Evidence from ALMA observations.
o	Calibrator J1709-3525 not identified.
o	Texte: <[CSB2017] G345.50M> N=1, <[CSB2017] G345.50S> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSB2019]
[CSB2019]	(Crnojevic+Sand+Bennet+, 2019)
Write:	<<[CSB2019] CenA-MM17-DwNN>>
N:	2
Object:	Dwarf G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Magellan Clay telescope Megacam observations of N=2 dwarf galaxies near Centaurus A, as part of the Panoramic Imaging Survey of Centaurus and Sculptor (PISCeS). See also [CSC2014], for other dwarf galaxies (confirmed and candidates) near Centaurus A.
in source:	Cen A = NGC 5128
Ref:	=2019ApJ...872...80C
by	CRNOJEVIC D. , SAND D.J., BENNET P., PASETTO S., SPEKKENS K., CALDWELL N., GUHATHAKURTA P., McLEOD B., SETH A., SIMON J.D., STRADER J., TOLOBA E.
	Astrophys. J., 872, 80-80 (2019)
	The faint end of the Centaurus A satellite luminosity function.
o	Sources DwNN-C16 are [CSC2014] CenA-MM-DwNN (Nos 10-13) in SIMBAD.
o	Fig. 1, Table 1: <[CSB2019] CenA-MM17-DwNN> (Nos Dw10-Dw11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSB98]
[CSB98]	(Crampton+Schechter+Beuzit, 1998)
Write:	<<[CSB98] G>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Note:	Table 1: N=1 galaxy, 'G', the lensing galaxy of the gravitational lensed system SBSG 1520+530. See also [CVS97], [FCK2002].
in source:	SBSG 1520+530
Ref:	=1998AJ....115.1383C
by	CRAMPTON D. , SCHECHTER P.L., BEUZIT J.-L.
	Astron. J., 115, 1383-1387 (1998)
	Detection of the galaxy lensing the doubly imaged quasar SBS 1520+530.
o	SBS 1520+530 = SBSG 1520+530. Components A, B, NW and SW = [CVS97] A, B, NW and SW.
o	Table 1: <[CSB98] G> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSC2006]
[CSC2006]	(Chen+Sanchawala+Chiu, 2006)
Write:	<<[CSC2006] NN>>
N:	34
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	ROSAT X-ray point-sources are identified as W UMa variable stars found in the All-Sky Automated Survey (ASAS).
Ref:	=2006AJ....131..990C
by	CHEN W.P. , SANCHAWALA K., CHIU M.C.
	Astron. J., 131, 990-993 (2006)
	W Ursae Majoris contact binary variables as X-ray sources.
o	Table 1: <[CSC2006] NN> (Nos 1-34).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSC2014]
[CSC2014]	(Crnojevic+Sand+Caldwell+, 2014)
Write:	<<[CSC2014] CenA-MM-DwNN>> <<[CSC2014] CenA-MM-DwNN-C16>> (not recognised by Simbad, but found in literature)
N:	13
Object:	Dwarf G + Poss. Dwarf G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Magellan Clay telescope Megacam observations of N=13 faint dwarf galaxies near Centaurus A, as part of the Panoramic Imaging Survey of Centaurus and Sculptor (PISCeS). See also [CSB2019] for additional dwarf galaxies near Centaurus A. See also [SCS2014] for a similar study near NGC 253.
in source:	Cen A = NGC 5128
Ref:	=2014ApJ...795L..35C
by	CRNOJEVIC D. , SAND D.J., CALDWELL N., GUHATHAKURTA P., McLEOD B., SETH A., SIMON J.D., STRADER J., TOLOBA E.
	Astrophys. J., 795L, 35 (2014)
	Discovery of a close pair of faint dwarf galaxies in the halo of Centaurus A.
o	Fig. 2, Table 1: <[CSC2014] CenA-MM-DwN> (Nos Dw1-Dw2).
Ref:	=2016ApJ...823...19C
by	CRNOJEVIC D. , SAND D.J., SPEKKENS K., CALDWELL N., GUHATHAKURTA P., McLEOD B., SETH A., SIMON J.D., STRADER J., TOLOBA E.
	Astrophys. J., 823, 19-19 (2016)
	The extended halo of Centaurus A: uncovering satellites, streams, and substructures.
o	Fig. 4, Tables 1+3: <[CSC2014] CenA-MM-DwN> (Nos Dw3-Dw13). Fig. 4, Paragr. 4.4: <[CSS2016b] Cloud S> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSC85]
[CSC85]	(Crampton+Schade+Cowley, 1985)
Write:	<<[CSC85] HHMM.M+DDNNA>>
N:	455
Object:	Poss. QSO + WD + * (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Note:	The 1950 right ascension are rounded, not truncated. 'NN' stands for hundredth of degree See also [CR82], [CP83], [CC87], [CCH87], [CCS88], [CCH90], [CCH91], [CCH92], [CGC97]
Ref:	=1985AJ.....90..987C
by	CRAMPTON D. , SCHADE D., COWLEY A.P.
	Astron. J., 90, 987-997 (1985)
	Quasar candidates from grens plates.
o	1950 right ascension are rounded, not truncated, Format HHMM.M+DDNNA: NN hundredth of °
o	<[CSC85] HHMM.M+DDNNA> N=455
=E=	Catalogue in electronic form as VII/143
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSD2012]
[CSD2012]	(Cook+Seth+Dale+, 2012) (Not yet in Simbad)
Write:	<<[CSD2012] {NGC\|UGC\|IC} NNNN NN>> <<[CSD2012] UGC a292 10>>
N:	44
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	N=44 star clusters with an age less than 100Myr, in a sample of nearby galaxies selected from the ACS Nearby Galaxy Survey Treasury (ANGST).
Ref:	=2012ApJ...751..100C
by	COOK D.O. , SETH A.C., DALE D.A., JOHNSON L.C., WEISZ D.R., FOUESNEAU M., OLSEN K.A.G., ENGELBRACHT C.W., DALCANTON J.J.
	Astrophys. J., 751, 100 (2012)
	The ACS nearby galaxy survey treasury. X. Quantifying the star cluster formation efficiency of nearby dwarf galaxies.
o	Table 2: <[CSD2012] NGC NNNN NN>, <[CSD2012] UGC NNNN NN>, <[CSD2012] IC NNNN NN>, <[CSD2012] UGC A292 10>, N=44.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSD2013]
[CSD2013]	(Castelletti+Supan+Dubner+, 2013)
Write:	<<[CSD2013] A>>
N:	2
Object:	Clump (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	Discovery of N=2 molecular clouds in the vicinity of HESS J1818-154. Use of Galactic Ring Survey 13CO(1-0) line data.
in source:	SNR G015.4+00.1
Ref:	=2013A&A...557L..15C
by	CASTELLETTI G. , SUPAN L., DUBNER G., JOSHI B.C., SURNIS M.P.
	Astron. Astrophys., 557L, 15-15 (2013)
	A hadronic scenario for HESS J1818-154.
o	Figure 1b: <[CSD2013] A> (Nos A and B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSD91]
[CSD91]	(Corbelli+Salpeter+Dickey, 1991)= (Ab) = (Af) = (Cb) = (Cf)
Write:	<<[CSD91] Ab NN>> <<[CSD91] Af NN>> <<[CSD91] Cb NN>> <<[CSD91] Cf NN>>
N:	30+49+18+34
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	In the format: Ab stands for bright galaxies in ACO 400 Af stands for faint galaxies in ACO 400 Cb stands for bright galaxies in Cancer cluster Cf stands for faint galaxies in Cancer cluster
in source:	ACO 400
in source:	NAME Cnc Cluster
Ref:	=1991ApJ...370...49C
by	CORBELLI E. , SALPETER E.E., DICKEY J.M.
	Astrophys. J., 370, 49-59 (1991)
	The joint far-infrared-optical luminosity function for spiral galaxies and data for the Abell 400 and Cancer clusters.
o	Table 2: <[CSD91] Ab NN> (Nos 1-30), <[CSD91] Af NN> (Nos 1-49), <[CSD91] Cb NN> (Nos 1-18), <[CSD91] Cf NN> (Nos 1-34)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSE2007]
[CSE2007]	(Comito+Schilke+Endesfelder+, 2007)
Write:	<<[CSE2007] HC>> <<[CSE2007] HCN>>
N:	3
Object:	Hot Core (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Plateau de Bure Interferomter observations of the [HW84] 2 region in Cep A: A Hot Core or Condensation was observed in 2005ApJ...628L..61M, and 2 independant condensations are found here.
in source:	NAME Cep A
Ref:	=2007A&A...469..207C
by	COMITO C. , SCHILKE P., ENDESFELDER U., JIMENEZ-SERRA I., MARTIN-PINTADO J.
	Astron. Astrophys., 469, 207-211 (2007)
	High-resolution study of a star-forming cluster in the Cepheus A HW2 region.
o	Fig.1: <[CSE2007] HC> N=1, <[CSE2007] HCN> (Nos HC2, HC3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSE2021]
[CSE2021]	(Chen+Steidel+Erb+, 2021)
Write:	<<[CSE2021] QHHMM-BXNNN-CSNN>>
N:	11
Object:	G (SIMBAD class: Galaxy)
Note:	Keck KCWI observations of N=11 continuum-detected serendipitous galaxies, as part of the Keck Baryonic Structure Survey (KBSS).
Ref:	=2021MNRAS.508...19C
by	CHEN Y. , STEIDEL C.C., ERB D.K., LAW D.R., TRAINOR R.F., REDDY N.A., SHAPLEY A.E., PAHL A.J., STROM A.L., LAMB N.R., LI Z., RUDIE G.C.
	Mon. Not. R. Astron. Soc., 508, 19-43 (2021)
	The KBSS-KCWI survey: the connection between extended Ly α haloes and galaxy azimuthal angle at z ~ 2-3.
o	Table 1: <[CSE2021] QHHMM-BXNNN-CSNN> N=11.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSE99]
[CSE99]	(Cotera+Simpson+Erickson+, 1999)
Write:	<<[CSE99] HHMMSS.s+DDMMSS>> <<[CSE99] Star H2-A>>
N:	6+2
Object:	* (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Note:	Table 1: format 'HHMMSS.s+DDMMSS', N=6 new emission-line sources coincident with stars, within 20pc of Sgr A West. [CSE99] 174218.2-285453, coincident with the peak of emission of [HJB85] Sgr A-H2, is also referred as 'Star H2-A', and there is a second star [HJB85] Sgr A-H2, referred as 'Star H2-B'. Maps Figs 2, 4, 6, 7. NAME in Table 1 is the name of the corresponding radio region. See also [HJB85] and [CEC96].
in source:	NAME Gal Center
Ref:	=1999ApJ...510..747C
by	COTERA A.S. , SIMPSON J.P., ERICKSON E.F., COLGAN S.W.J., BURTON M.G., ALLEN D.A.
	Astrophys. J., 510, 747-758 (1999)
	Isolated hot stars in the Galactic Center vicinity.
o	Table 1: <[CSE99] HHMMSS.s-DDMMSS> N=6. Fig.6: <[CSE99] Star H2-A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSF2006]
[CSF2006]	(Clocchitti+Schmidt+Filippenko+, 2006) (Not yet in Simbad)
Write:	<<[CSF2006] SN YYYYA NN>>
N:	22+21+39+17+34
Object:	* (SIMBAD class: Star)
Note:	Standard stars in the fields of SN 1999M, SN 1999N, SN 1999Q, SN 1999S, SN 1999U.
Ref:	=2006ApJ...642....1C
by	CLOCCHIATTI A. , SCHMIDT B.P., FILIPPENKO A.V., CHALLIS P., COIL A.L., COVARRUBIAS R., DIERCKS A., GARNAVICH P., GERMANY L., GILLILAND R., HOGAN C., JHA S., KIRSHNER R.P., LEIBUNDGUT B., LEONARD D., LI W., MATHESON T., PHILLIPS M.M., PRIETO J.L., REISS D., RIESS A.G., SCHOMMER R., SMITH R.C., SODERBERG A., SPYROMILIO J., STUBBS C., SUNTZEFF N.B., TONRY J.L., WOUDT P.
	Astrophys. J., 642, 1-21 (2006)
	Hubble Space Telescope and ground-based observations of type Ia supernovae at redshift 0.5: cosmological implications.
o	Figs 11-15, Tables 3-7: <[CSF2006] SN YYYYA NN> N=22+21+39+17+34.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSF2007]
[CSF2007]	(Capezzali+Spogli+Fiorucci+, 2007)
Write:	<<[CSF2007] CN>>
N:	6
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	BVRI photometry at the 0.35m telescope of the Porziano Observatory of VW Vul and N=6 comparison stars.
Ref:	=2007IBVS.5749....1C
by	CAPEZZALI D. , SPOGLI C., FIORUCCI M., CIPRINI S., NUCCIARELLI G., MANCINELLI V., BRUNOZZI P., FAGOTTI P., BRANDONI L., ROCCHI G.
	IAU Inform. Bull. Var. Stars, 5749, 1-4 (2007)
	BVRI photometry of VW Vul and new comparison stars.
o	Table 1: <[CSF2007] CN> (Nos C1-C6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSF2018]
[CSF2018]	(Chiti+Simon+Frebel+, 2018)
Write:	<<[CSF2018] FF-N-NNNN>> <<[CSF2018] FF_N_NNNN>> (not recognised by Simbad, but found in literature)
N:	26+100
Object:	* (SIMBAD class: Star)
Note:	Magellan Clay 6.5m telescope M2FS and Magellan Baade 6.5m telescope MagE spectroscopic observations of N=26+100 metal-poor stars in the Sculptor Dwarf Spheroidal Galaxy.
in source:	NAME Sculptor dSph
Ref:	=2018ApJ...856..142C
by	CHITI A. , SIMON J.D., FREBEL A., THOMPSON I.B., SHECTMAN S.A., MATEO M., BAILEY J.I., CRANE J.D., WALKER M.
	Astrophys. J., 856, 142-142 (2018)
	Detection of a population of carbon-enhanced metal-poor stars in the Sculptor dwarf spheroidal galaxy.
o	Tables 5-6: <[CSF2018] FF-N-NNNN> N=26+100.
=E=	Catalogue in electronic form as <J/ApJ/856/142/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSG2000]
[CSG2000]	(Cole+Smecker-Hane+Gallagher, 2000)
Write:	<<[CSG2000] Red NN>> <<[CSG2000] NNNNNN>>
N:	40+16964
Object:	* (SIMBAD class: Star)
Note:	Table 1: N=40 red giants among (Nos 1-51). Table 6: N=16964 stars, used in Stromgren photometry.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2000AJ....120.1808C
by	COLE A.A. , SMECKER-HANE T.A., GALLAGHER III J.S.
	Astron. J., 120, 1808-1829 (2000)
	The metallicity distribution function of red giants in the Large Magellanic Cloud.
o	Table 1: <[CSG2000] Red NN> N=40 among (Nos 1-51). Table 6: <[CSG2000] NNNNNN> N=16964.
=E=	Catalogue in electronic form as J/AJ/120/1808
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSG2002]
[CSG2002]	(Cannon+Skillman+Garnett+, 2002)= ([CSG2002a])
Write:	<<[CSG2002] WW NN>>
N:	15
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of Zw I 18. See also [HT95].
in source:	Zw I 18 = Mrk 116
Ref:	=2002ApJ...565..931C
by	CANNON J.M. , SKILLMAN E.D., GARNETT D.R., DUFOUR R.J.
	Astrophys. J., 565, 931-940 (2002)
	Dust in I Zw 18 from Hubble Space Telescope narrowband imaging.
o	Table 3: [HT95] HII 16 not in the [HT95] list, = [HT95] HII 4 (information from J. Cannon).
o	Fig.2, Table 3: <[CSG2002] WW NN> (Nos NW 1-2, SE 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSG2002a]
[CSG2002a]	(Cannon+Skillman+Garnett+, 2002)
*****	Avoid the usage of [CSG2002a], prefer [CSG2002]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSG2002b]
[CSG2002b]	(Campana+Stella+Gastaldello+, 2002)
Write:	<<[CSG2002b] JHHMMSS.s+DDMMSS>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of SAX J1808.4-3658 field. 2 new faint sources are observed. See also [GSG99], [RCM98], [SCM2000].
Ref:	=2002ApJ...575L..15C
by	CAMPANA S. , STELLA L., GASTALDELLO F., MEREGHETTI S., COLPI M., ISRAEL G.L., BURDERI L., DI SALVO T., ROBBA N.R.
	Astrophys. J., 575, 15-19 (2002)
	An XMM-newton study of the 401 Hz accreting pulsar SAX J1808.4-3658 in quiescence.
o	<[CSG2002b] JHHMMSS.s+DDMMSS> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSG2005]
[CSG2005]	(Collins+Shull+Giroux+, 2005)
Write:	<<[CSG2005] QSO J1305-1033 abs N.NNN>> <<[CSG2005] QSO J0057-2222 abs N.NNNN>>
N:	2
Object:	Absorber
Note:	HST STIS and FUSE spectroscopic data of QSOs. Absorber systems are observed in PKS 1302-102 = QSO J1305-1033 and Ton S 180 = QSO J0057-2222.
Ref:	=2005ApJ...623..196C
by	COLLINS J.A. , SHULL J.M., GIROUX M.L.
	Astrophys. J., 623, 196-212 (2005)
	Highly ionized high-velocity clouds: hot intergalactic medium or galactic halo?
o	Paragr.3.6: z = 0.07118 is a misprint for 0.07188 ([STS2004] QSO J1119+2119 abs 0.07188)
o	Paragr.3.8: <[CSG2005] QSO J1305-1033 abs 0.099> N=1. Paragr.3.9: <[CSG2005] QSO J0057-2222 abs 0.0184> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSG2012]
[CSG2012]	(Cooke+Sullivan+Gal-Yam+, 2012)
Write:	<<[CSG2012] SN JHHMM+DDMM>> <<[CSG2012] SN HHMM+DDMM>> (not recognised by Simbad, but found in literature)
N:	2
Object:	SN (SIMBAD class: Supernova = SuperNova)
Stat:	is completely incorporated in Simbad
Note:	Keck I LRIS spectroscopy of N=2 supernovae in the CFHTLS Deep Fields.
Ref:	=2012Natur.491..228C
by	COOKE J. , SULLIVAN M., GAL-YAM A., BARTON E.J., CARLBERG R.G., RYAN-WEBER E.V., HORST C., OMORI Y., DIAZ G.
	Natur, 491, 228-231 (2012)
	Superluminous supernovae at redshifts of 2.05 and 3.90.
o	Table 1: <[CSG2012] SN JHHMM+DDMM> N=2.
=E=	Catalogue in electronic form as J/other/Nat/491.228
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSH2002]
[CSH2002]	(Crampton+Schade+Hammer+, 2002)
Write:	<<[CSH2002] IN>> <<[CSH2002] Lensed G>>
N:	3+1
Object:	Lensed Image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Stat:	is completely incorporated in Simbad
Note:	HST observations. Lensed images of the gravitational lens CFRS 03.1077, arc (I0) and counterimages (I1 and I2), the lensed galaxy has a redshift of 2.941.
Ref:	=2002ApJ...570...86C
by	CRAMPTON D. , SCHADE D., HAMMER F., MATZKIN A., LILLY S.J., LE FEVRE O.
	Astrophys. J., 570, 86-91 (2002)
	The gravitational lens CFRS 03.1077.
o	Text: <[CSH2002] Lensed G> N=1. Fig.5: <[CSH2002] AN> (Nos I0, I1, I2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSH2004]
[CSH2004]	(Connoly+Sloan DSSC+Holvorcem+, 2004)
Write:	<<[CSH2004] JHHMMSS.s+DDMMSS>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	SDSS observations. Host galaxy of SN 2004AR.
Ref:	=2004IAUC.8302....1C
by	CONNOLLY A. , (The Sloan Digital Sky Survey Collaboration), HOLVORCEM P., SCHWARTZ M.
	IAU Circ., 8302, 1-None (2004)
	Supernovae 2004ar, 2004as, and 2004at.
o	<[CSH2004] JHHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSH2009]
[CSH2009]	(Collins+Stott+Hilton+, 2009) (Not yet in Simbad)
Write:	<<[CSH2009] JHHMM BCG>>
N:	5
Object:	BCG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	N=5 brightest cluster galaxies in 5 of the most distant clusters in their respective X-ray surveys.
Ref:	=2009Natur.458..603C
by	COLLINS C.A. , STOTT J.P., HILTON M., KAY S.T., STANDFORD S.A., DAVIDSON M., HOSMER M., HOYLE B., LIDDLE A., LLOYD-DAVIES E., MANN R.G., MEHRTENS N., MILLER C.J., NICHOL R.C., ROMER A.K., SAHLEN M., VIANA P.T.P., WEST M.J.
	Natur, 458, 603-606 (2009)
	Early assembly of the most massive galaxies.
o	Table 1: <[CSH2009] JHHMM {BCG}> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSH96]
[CSH96]	(Cowie+Songaila+Hu+, 1996)
Write:	<<[CSH96] SSA 13 NNN>> <<[CSH96] SSA 22 NNN>>
N:	174+211
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	objects in 2 Hawaii Deep Survey fields, SSA 13 and 22 (SSA fields are defined in 1991ApJ...369...79L). N=174 among (Nos 0-175) in SSA 13. N=210 among (Nos 0-218) in SSA 22. Finding charts in Fig. 1(a) and (b). See also [CGH94] and [SCH94]
in source:	SSA 13
in source:	SSA 22
Ref:	=1996AJ....112..839C
by	COWIE L.L. , SONGAILA A., HU E.M., COHEN J.G.
	Astron. J., 112, 839-864 (1996)
	New insight on Galaxy formation and evolution from Keck spectroscopy of the Hawaii deep fields.
o	Table 1(a): <[CSH96] SSA 13 NNN> (Nos 0-173). Table 1(b): <[CSH96] SSA 22 NNN> (Nos 0-218)
Ref:	=2016MNRAS.456.1195H
by	HARRISON C.M. , ALEXANDER D.M., MULLANEY J.R., STOTT J.P., SWINBANK A.M., ARUMUGAM V., BAUER F.E., BOWER R.G., BUNKER A.J., SHARPLES R.M.
	Mon. Not. R. Astron. Soc., 456, 1195-1220 (2016)
	The KMOS AGN Survey at High redshift (KASHz): the prevalence and drivers of ionized outflows in the host galaxies of X-ray AGN.
o	Table A.1: <[CSH96] SSA 22 NNN> (Nos 141) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CSI
CSI	(Catalog of Stellar Identif.)
Write:	<<CSI +DD NNNNN NN>> <<CSI +DD-HHMMm NN>>
N:	494946
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Compilation updated by the CDS (Centre de Donnees astronomiques de Strasbourg). The CSI number is built from the BD or southern extension number otherwise from the 1950 equatorial coordinates 1981A&AS...43..259O: Microfiche edition of CSI See also: 'Le Centre de Donnees des Amas de Galaxies (CEDAG)' (IAU Coll. 64, Strasbourg 1981, 'Automated Data Retrieval in Astronomy', C. Jaschek and W. Heintz, eds, Reidel, Dordrecht, p. 265-271)
Ref:	=1973BICDS...4...27J
by	JUNG J. , BISCHOFF M., OCHSENBEIN F.
	Bull. Inf. Centre Donnees Stellaires, 4, 27-35 (1973)
	The Catalogue of Stellar Identifications.
o	Table 1: <CSI +DD NNNNN NN>
Ref:	=1981A&AS...43..259O
by	OCHSENBEIN F. , BISCHOFF M., EGRET D.
	Astron. Astrophys., Suppl. Ser., 43, 259-264 (1981)
	Microfiche edition of CSI.
o	<CSI +DD NNNNN NN> N=494946
Ref:	=1983BICDS..24..109E
by	EGRET D.
	Bull. Inf. Centre Donnees Stellaires, 24, 109-123 (1983)
	S.I.M.B.A.D story: a description of the data base of the Strasbourg stellar data center.
o	<CSI +DD NNNNN NN>
=E=	Catalogue in electronic form as IV/9
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSI2002]
[CSI2002]	(Chapman+Smail+Ivison+, 2002)= ([CSI2002a])
Write:	<<[CSI2002] CFN1 64 JN>> <<[CSI2002] FN1 40 JN>>
N:	2+3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Observations of 2 FIRBACK sources. FIRBACK CFN1 64 is a pair of galaxies with 2 components J1 and J2 separated by 2".4. FIRBACK FN1 40 is a faint galaxy J1 with a possible close companion J2 at 2".3 and a third optical bright galaxy J3 at 3".6 from J1.
in source:	FIRBACK CFN1 064
in source:	FIRBACK FN1 040
Ref:	=2002ApJ...573...66C
by	CHAPMAN S.C. , SMAIL I., IVISON R.J., HELOU G., DALE D.A., LAGACHE G.
	Astrophys. J., 573, 66-74 (2002)
	Optically faint counterparts to the infrared space observatory FIRBACK 170 micron population: discovery of cold, luminous galaxies at high redshift.
o	Table 1: Objects FN1-40 and FN1-64 = respectively FIRBACK FN1 40 and FIRBACK CFN1 64.
o	Fig.1, text: <[CSI2002] CFN1 64 JN> (Nos J1-J2), <[CSI2002] FN1 40 JN> (Nos J1-J3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSI2002a]
[CSI2002a]	(Chapman+Smail+Ivison+, 2002)
*****	Avoid the usage of [CSI2002a], prefer [CSI2002]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSI2002b]
[CSI2002b]	(Chapman+Smail+Ivison+, 2002)= (SMM)
Write:	<<[CSI2002b] SMM JHHMMm+DDMM>>
N:	5
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	Search for optically bright counterparts to submillimeter-selected sources.
Ref:	=2002MNRAS.335L..17C
by	CHAPMAN S.C. , SMAIL I., IVISON R.J., BLAIN A.W.
	Mon. Not. R. Astron. Soc., 335, 17-21 (2002)
	The effect of lensing on the identification of SCUBA galaxies.
o	Table 1, last col.: N2 850.1 = [SFD2002] N2 1, ERO: M12 = [BCS99b] Cl 0024+16 M12, ERO: N4 = [BCS99b] Cl 0440+02 N4, HDF 850.1 = [HSD98] F850.1. SSA22 850.2 is one of the [CLS2001] object, but which one?
o	Table 1: <[CSI2002b] SMM JHHMMm+DDMM> N=5. Table 1: <[BCS99b] Cl 0024+16 MNN> (No. M12) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSI2006]
[CSI2006]	(Chen+Shen+Imai+, 2006) (Not yet in Simbad)
Write:	<<[CSI2006] N NNN>>
N:	110+110+105
Object:	SiO Maser (SIMBAD class: Maser)
Note:	VLBA observations of SiO maser features around VX Sgr at 3 different epochs.
in source:	V* VX Sgr
Ref:	=2006ApJ...640..982C
by	CHEN X. , SHEN Z.-Q., IMAI H., KAMOHARA R.
	Astrophys. J., 640, 982-994 (2006)
	Inward motions of the compact SiO masers around VX Sagittarii.
o	Table 2: <[CSI2006] 1 NNN> (Nos 1-110). Table 3: <[CSI2006] 2 NNN> (Nos 1-110). Table 4: <[CSI2006] 3 NNN> (Nos 1-105).
=E=	Catalogue in electronic form as J/ApJ/640/982
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSI2016]
[CSI2016]	(Chen+Smail+Ivison+, 2016)
Write:	<<[CSI2016] UDS.NNNN IDN>>
N:	330+248
Object:	(Rad) + (IR) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=330+248 candidate counterparts of SCUBA-2 Cosmology Legacy Survey (S2CLS) in the UKIDSS UDS field. Use of UKIDSS UDS DR8, CFHT Megacam, SXDS, Spitzer SpUDS, and VLA data.
Ref:	=2016ApJ...820...82C
by	CHEN C.-C. , SMAIL I., IVISON R.J., ARUMUGAM V., ALMAINI O., CONSELICE C.J., GEACH J.E., HARTLEY W.G., MA C.-J., MORTLOCK A., SIMPSON C., SIMPSON J.M., SWINBANK A.M., ARETXAGA I., BLAIN A., CHAPMAN S.C., DUNLOP J.S., FARRAH D., HALPERN M., MICHALOWSKI M.J., VAN DER WERF P., WILKINSON A., ZAVALA J.A.
	Astrophys. J., 820, 82 (2016)
	The SCUBA-2 cosmology legacy survey: multiwavelength counterparts to 10^{3} submillimeter galaxies in the UKIDSS-UDS field.
o	Tables 3-4: <[CSI2016] UDS.NNNN IDN> N=330+248.
=E=	Catalogue in electronic form as J/ApJ/820/82
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CSIMon
CSIMon	(Coordinated Synoptic Investigation of NGC 2264)
Write:	<<CSIMon -NNNNNN>>
N:	146855
Object:	* (SIMBAD class: Star)
Note:	We have photometrically monitored thousands of stars in and near the NGC 2264 cluster, as part of the Coordinated Synoptic Investigation of NGC 2264: http://csi2264.ipac.caltech.edu/ This catalog is a comprehensive list of optical and infrared objects found in our monitoring field.
in source:	NGC 2264
Ref:	=2014AJ....147...82C
by	CODY A.M. , STAUFFER J., BAGLIN A., MICELA G., REBULL L.M., FLACCOMIO E., MORALES-CALDERON M., AIGRAIN S., BOUVIER J., HILLENBRAND L.A., GUTERMUTH R., SONG I., TURNER N., ALENCAR S.H.P., ZWINTZ K., PLAVCHAN P., CARPENTER J., FINDEISEN K., CAREY S., TEREBEY S., HARTMANN L., CALVET N., TEIXEIRA P., VRBA F.J., WOLK S., COVEY K., POPPENHAEGER K., GUNTHER H.M., FORBRICH J., WHITNEY B., AFFER L., HERBST W., HORA J., BARRADO D., HOLTZMAN J., MARCHIS F., WOOD K., GUIMARAES M.M., LILLO BOX J., GILLEN E., McQUILLAN A., ESPAILLAT C., ALLEN L., D'ALESSIO P., FAVATA F.
	Astron. J., 147, 82 (2014)
	CSI 2264: simultaneous optical and infrared light curves of young disk-bearing stars in NGC 2264 with CoRoT and Spitzer–Evidence for multiple origins of variability.
o	Tables 3-4: <CSIMon-NNNNNN> N=162.
Ref:	=2014A&A...570A..82V
by	VENUTI L. , BOUVIER J., FLACCOMIO E., ALENCAR S.H.P., IRWIN J., STAUFFER J.R., CODY A.M., TEIXEIRA P.S., SOUSA A.P., MICELA G., CUILLANDRE J.-C., PERES G.
	Astron. Astrophys., 570A, 82-82 (2014)
	Mapping accretion and its variability in the young open cluster NGC 2264: a study based on u-band photometry.
o	Tables 2-4: <CSIMon-NNNNNN> N=757. IPAC, California Institute of Technology
=E=	Catalogue in electronic form as J/A+A/570/A82
=E=	Catalogue in electronic form as <J/AJ/147/82/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: Csk
Csk	(Coalsack)
*****	Avoid the usage of Csk, prefer [JHR80]
Origin	of the Acronym: L (1998AJ....116.2476P)
Details on Acronym: [CSK2004]
[CSK2004]	(Chandra+Swarup+Kulkarni+, 2004)
Write:	<<[CSK2004] N>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	HI absorption measurements:
Note:	N=3 radio sources in the field of B2 0902+34.
Ref:	=2004JApA...25...57C
by	CHANDRA P. , SWARUP G., KULKARNI V.K., KANTHARIA N.G.
	J. Astrophys. Astron., 25, 57-65 (2004)
	Associated HI absorption in the z=3.4 radio galaxy B2 0902+343 observed with the GMRT.
o	Table 2: <[CSK2004] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSK2007]
[CSK2007]	(Colgan+Schultz+Kaufman+, 2007)
Write:	<<[CSK2007] SSs-MSS>>
N:	13
Object:	H2 (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST NICMOS observations of shocked H2 knots in Orion. See also [OW94].
in source:	NAME Orion Nebula
Ref:	=2007ApJ...671..536C
by	COLGAN S.W.J. , SCHULTZ A.S.B., KAUFMAN M.J., ERICKSON E.F., HOLLENBACH D.J.
	Astrophys. J., 671, 536-545 (2007)
	NICMOS observations of shocked H_{2} in Orion.
o	Table 1: <[CSK2007] SSs-MSS> N=13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSK2011]
[CSK2011]	(Cohen+Sarajedini+Kinemuchi+, 2011)
Write:	<<[CSK2011] NNNNN>>
N:	10811
Object:	*
Note:	CTIO Yale 1.0m telescope observations of the Galactic globular cluster NGC 6101.
in source:	NGC 6101
Ref:	=2011ApJ...727....9C
by	COHEN R.E. , SARAJEDINI A., KINEMUCHI K., LEITON R.
	Astrophys. J., 727, 9 (2011)
	The unusual RR Lyrae population of NGC 6101.
o	Table 2: <Cl* NGC 6101 Saw VNN> (Nos 16-22) added. Table 3: <[CSK2011] NNNNN> N=10811 among (Nos 1-11032).
=E=	Catalogue in electronic form as <J/ApJ/727/9/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSK2012]
[CSK2012]	(Crockett+Shabala+Kaviraj+, 2012)
Write:	<<[CSK2012] NNN>>
N:	111
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	HST WFC3 observations of N=111 sources in the field of the inner filament of Centaurus A. Use of archival HST ACS data.
in source:	Cen A = NGC 5128
Ref:	=2012MNRAS.421.1603C
by	CROCKETT R.M. , SHABALA S.S., KAVIRAJ S., ANTONUCCIO-DELOGU V., SILK J., MUTCHLER M., O'CONNELL R.W., REJKUBA M., WHITMORE B.C., WINDHORST R.A.
	Mon. Not. R. Astron. Soc., 421, 1603-1623 (2012)
	Triggered star formation in the inner filament of Centaurus A.
o	Table A1: <[CSK2012] NNN> (Nos 1-111).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CSL
CSL	(Capodimonte-Sternberg Lens)
Write:	<<CSL NA>>
N:	4+2
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=4 lens candidates discovered in the OACDF (Osservatorio Astronomico di Capodimonte Deep Field). Object 1 is an extragalactic double source which could be the first case of gravitational lensing by a cosmic string.
Ref:	=2003MNRAS.343..353S
by	SAZHIN M. , LONGO G., CAPACCIOLI M., ALCALA J.M., SILVOTTI R., COVONE G., KHOVANSKAYA O., PAVLOV M., PANNELLA M., RADOVICH M., TESTA V.
	Mon. Not. R. Astron. Soc., 343, 353-359 (2003)
	CSL-1: chance projection effect or serendipitous discovery of a gravitational lens induced by a cosmic string.
o	<CSL NA> (Nos 1-4, 1A, 1B).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CSL2007]
[CSL2007]	(Chen+Su+Liu+, 2007)
Write:	<<[CSL2007] Clump A>>
N:	2
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SMA 223 and 654GHz observations toward the UC HII region [BNM96] 240.315+0.071. The continuum emission is resolved in N=2 clumps.
in source:	[BNM96] 240.315+0.071
Ref:	=2007ApJ...654L..87C
by	CHEN H.-R. , SU Y.-N., LIU S.-Y., HUNTER T.R., WILNER D.J., ZHANG Q., LIM J., HO P.T.P., OHASHI N., HIRANO N.
	Astrophys. J., 654L, 87-90 (2007)
	654 GHz continuum and C^{18}O(6-5) observations of G240.31+0.07 with the submillimeter array.
o	Fig.1, text: <[CSL2007] Clump A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSL2009]
[CSL2009]	(Corbally+Straizys+Laugalys, 2009)
Write:	<<[CSL2009] CSL N>>
N:	8
Object:	Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Stat:	is completely incorporated in Simbad
Note:	Steward Observatory 2.3m telescope spectroscopy of the North America and Pelican nebulae region.
Ref:	=2009BaltA..18..111C
by	CORBALLY C.J. , STRAIZYS V., LAUGALYS V.
	BaltA, 18, 111-139 (2009)
	Spectral analysis of YSOs and other emission-line stars in the North America and Pelican nebulae region.
o	Tables 1, 3: <[CSL2009] CSL N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSL2018]
[CSL2018]	(Collier+Smith+Lucey, 2018)
Write:	<<[CSL2018] J0403 A>> <<[CSL2018] J0403 system>>
N:	2+1
Object:	Grav. lensed image of a G + Grav. lens system (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=2 gravitationally lensed images in N=1 gravitational lens system. Use of archival VLT MUSE data.
Ref:	=2018MNRAS.478.1595C
by	COLLIER W.P. , SMITH R.J., LUCEY J.R.
	Mon. Not. R. Astron. Soc., 478, 1595-1600 (2018)
	A new strong-lensing galaxy at z= 0.066: another elliptical galaxy with a lightweight IMF.
o	<[CSL2018] J0403 system> N=1. Fig. 1: <[CSL2018] J0403 A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CSM
CSM	(Coelho+Shafter+Misselt)
*****	Avoid the usage of CSM, prefer [CSM2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CSM2008]
[CSM2008]	(Coelho+Shafter+Misselt, 2008)= (CSM)
Write:	<<[CSM2008] YYYY-N>> <<[CSM2008] 2006-6>>
N:	13
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Stat:	is completely incorporated in Simbad
Note:	Steward Observatory 2.3m Bok telescope narrowband Halpha observations to search for novae in M 101.
in source:	M 101 = NGC 5457
Ref:	=2008ApJ...686.1261C
by	COELHO E.A. , SHAFTER A.W., MISSELT K.A.
	Astrophys. J., 686, 1261-1268 (2008)
	The rate and spatial distribution of novae in M101 (NGC 5457).
o	Table 2: <[CSM2008] YYYY-N> N=13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSM2011]
[CSM2011]	(Carlson+Sewilo+Meisner+, 2011)
Write:	<<[CSM2011] ANNN>>
N:	77
Object:	(NIR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	HST ACS, SMARTS ANDICAM, Spitzer IRAC and MIPS observations of N=77 sources in the star-forming cluster NGC 602. A letter is used as a prefix to the IRAC number given in col(1) of Table 4: Y => well-fit YSO; G => galaxy; S => star; K => single, naked star with Kurucz model; U => unknown nature (a prefix "A" is also used and stands for "all photometric data", in that case, prefer the usage of SSTNGC602). See also HSTNGC602, SSTNGC602
in source:	NGC 602
Ref:	=2011ApJ...730...78C
by	CARLSON L.R. , SEWILO M., MEIXNER M., ROMITA K.A., WHITNEY B., HORA J.L., CIGNONI M., SABBI E., NOTA A., SIRIANNI M., SMITH L.J., GORDON K., BABLER B., BRACKER S., GALLAGHER J.S., MEADE M., MISSELT K., PASQUALI A., SHIAO B.
	Astrophys. J., 730, 78 (2011)
	A panchromatic view of NGC 602: time-resolved star formation with the Hubble and Spitzer space telescopes.
o	Table 2: <HSTNGC602 JHHMMSS.sss+DDMMSS.ss> N=4535. Table 3, col(2): <SSTNGC602 JHHMMSS.ss+DDMMSS.s> N=497. Table 4, col(1): <[CSM2011] ANNN> N=77.
=E=	Catalogue in electronic form as <J/ApJ/730/78/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSM2017]
[CSM2017]	(Carraro+Sales Silva+Moni Bidin+, 2017)
Write:	<<[CSM2017] NNNNN>>
N:	31
Object:	* (SIMBAD class: Star)
Note:	CTIO SMARTS 1.0m telescope Y4KCAM photometry and Magellan IMACS spectroscopy of N=31 stars in a field toward the open cluster Tombaugh 1. See also [SCA2016].
in source:	Cl Tombaugh 1
Ref:	=2017AJ....153...99C
by	CARRARO G. , SALES SILVA J.V., MONI BIDIN C., VAZQUEZ R.A.
	Astron. J., 153, 99-99 (2017)
	Galactic structure in the outer disk: the field in the line of sight to the intermediate-age open cluster Tombaugh 1.
o	Table 2: <[CSM2017] NNNNN> N=31 among (Nos 6507-36132).
=E=	Catalogue in electronic form as <J/AJ/153/99/>
Details on Acronym: [CSM97]
[CSM97]	(Cowley+Schmidtke+McGrath+, 1997)
Write:	<<[CSM97] JHHMM.m+DDMM NN>>
N:	82
Object:	* (SIMBAD class: Star)
Note:	ROSAT HRI observations N=82 stars around 14 RX sources See also WHHW and WW
in source:	Magellanic Clouds:LMC = LMC
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1997PASP..109...21C
by	COWLEY A.P. , SCHMIDTKE P.C., McGRATH T.K., PONDER A.L., FERTIG M.R., HUTCHINGS J.B., CRAMPTON D.
	Publ. Astron. Soc. Pac., 109, 21-None (1997)
	Magellanic cloud X-ray sources observed with ROSAT.
o	EXO 0114.6-7361 = EXO 0114.6-7336
o	Figs 3-8: <[CSM97] JHHMM.m-DDMM NN> N=82
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSN2007]
[CSN2007]	(Coppin+Swinbank+Neri+, 2007) (Not yet in Simbad)
Write:	<<[CSN2007] LBG As>> <<[CSN2007] knot BN>>
N:	2+2
Object:	Part of G + Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Observations of the LBG system [SSR2007] LBG J213512.73-010143. N=2 components of the LBG, (Nos As, Bs), and N=2 images near the [SSR2007] Arc N, (Nos B1, B2).
Ref:	=2007ApJ...665..936C
by	COPPIN K.E.K. , SWINBANK A.M., NERI R., COX P., SMAIL I., ELLIS R.S., GEACH J.E., SIANA B., TEPLITZ H., DYE S., KNEIB J.-P., EDGE A.C., RICHARD J.
	Astrophys. J., 665, 936-943 (2007)
	A detailed study of gas and star formation in a highly magnified Lyman Break Galaxy at z = 3.07.
o	The LBG = [SSR2007] LBG J213512.73-010143.
o	Fig.1: <[CSN2007] LBG As> (Nos As, Bs), <[CSN2007] Knot AN> (Nos B1, B2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CSO
CSO	(Case univ., Stellar Obj.)
Write:	<<CSO NNNN>>
N:	1336
Object:	Blue Obj. (SIMBAD class: blue = Blue Object)
Note:	Identif. charts.
Ref:	=1983ApJS...51..171P
by	PESCH P. , SANDULEAK N.
	Astrophys. J., Suppl. Ser., 51, 171-182 (1983)
	The Case low-dispersion northern sky survey. I.
o	Table 1: <CasG NN> (Nos 1-71), Table 1A: <CasHII Z FFF-NNN a> N=4, Table 2: <CSO NN> (Nos 1-59), Table 3: <CBS NN> (Nos 1-28)
Ref:	=1984ApJS...55..517S
by	SANDULEAK N. , PESCH P.
	Astrophys. J., Suppl. Ser., 55, 517-532 (1984)
	The Case low-dispersion northern sky survey. II.
o	(Erratum) Erratum 1996 ApJS 103, p. 513
o	Table 1: <CasG NNN> (Nos 72-196), Table 1A: <CasHII Z FFF-NNN a> N=40, Table 2: <CSO NNN> (Nos 60-179), Table 3: <CBS NN> (Nos 29-66)
Ref:	=1986ApJS...60..543P
by	PESCH P. , SANDULEAK N.
	Astrophys. J., Suppl. Ser., 60, 543-549 (1986)
	The Case low-dispersion northern sky survey. III.
o	Table 1: <CasG NNN> (Nos 197-326), Table 1A: <CasHII Z FFF-NNN a> N=6, <CasHII HHMMSS.s+DDMM.m a> N=1, Table 2: <CSO NNN> (Nos 180-252), Table 3: <CBS NNN> (Nos 67-124)
Ref:	=1988ApJS...66..297P
by	PESCH P. , SANDULEAK N.
	Astrophys. J., Suppl. Ser., 66, 297-307 (1988)
	The Case low-dispersion northern sky survey. V.
o	Table 1: <CasG NNN> (Nos 753-895), Table 1A: <CasHII Z FFF-NNN a> N=20, <CasHII HHMMSS.s+DDMM.m a> N=3, Table 2: <CSO NNN> (Nos 253-401), Table 3: <CBS NNN> (Nos 125-160)
Ref:	=1989ApJS...70..163P
by	PESCH P. , SANDULEAK N.
	Astrophys. J., Suppl. Ser., 70, 163-171 (1989)
	The Case low-dispersion northern sky survey. VIII. A region centered in southern Bootes.
o	Table 1: <CasG NNN> (Nos 896-907), Table 2: <CSO NNN> (Nos 402-602), Table 3: <CBS NNN> (Nos 161-252)
Ref:	=1989ApJS...70..173S
by	SANDULEAK N. , PESCH P.
	Astrophys. J., Suppl. Ser., 70, 173-179 (1989)
	The Case low-dispersion northern sky survey. IX. A region centered in northern Bootes.
o	Table 1: <CasG NNN> (Nos 908-925), Table 2: <CSO NNN> (Nos 603-765), Table 3: <CBS NNN> (Nos 253-324)
Ref:	=1990ApJS...72..291S
by	SANDULEAK N. , PESH P.
	Astrophys. J., Suppl. Ser., 72, 291-301 (1990)
	The Case low-dispersion northern sky survey. XI. A region near the North Galactic Pole including SA 57.
o	Table 1: <CasG NNNN> (Nos 926-1019), Table 2: <CSO NNN> (Nos 766-881), Table 3: <CBS NNN> (Nos 325-350)
Ref:	=1991ApJS...76.1043P
by	PESCH P. , SANDULEAK N., STEPHENSON C.B.
	Astrophys. J., Suppl. Ser., 76, 1043-1053 (1991)
	The Case low-dispersion northern sky survey. XII. A region in southern Canes Venatici.
o	(Erratum) Erratum 1996 ApJS 102, p. 435, and 1996 ApJS 103, p. 513
o	Table 2: <CasG NNNN> (Nos 1020-1213), Table 3: <CasHII PGC NNNNN>, <CasHII PGC NNNNN a> N=3+12, Table 4: <CSO NNNN> (Nos 882-1038), Table 5: <CBS NNN> (Nos 351-382)
Ref:	=1992ApJS...82..471S
by	STEPHENSON C.B. , PESCH P., MacCONNELL D.J.
	Astrophys. J., Suppl. Ser., 82, 471-487 (1992)
	The case Low-Dispersion Northern Sky Survey. XIII. A region in central Bootes and Corona Borealis.
o	Table 1: <CasG NNNN> (Nos 1214-1351), Table 2:<CasHII PGC NNNNN a> N=4, Table 3: <CSO NNNN> (Nos 1039-1121), Table 4: <CBS NNN> (Nos 383-418)
Ref:	=1995ApJS...98...41P
by	PESCH P. , STEPHENSON C.B., MacCONNELL D.J.
	Astrophys. J., Suppl. Ser., 98, 41-67 (1995)
	The Case low-dispersion northern sky survey. XV. A region in Ursa Major and Canes Venatici.
o	(Erratum) Erratum 1996 ApJS 102, p. 435, and 1996 ApJS 103, p. 513
o	Table 1: <CasG NNNN> (Nos 1352-1579), Table 2: <CasHII PGC NNNNN> <CasHII PGC NNNNN a> <CasHII Anon a> N=7+34+2, Table 4: <CSO NNNN> (Nos 1122-1336), Table 5: <CBS NNN> (Nos 419-465)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CSO
CSO	(Caltech Submm Observatory)
*****	Avoid the usage of CSO, prefer [LSK98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CSO2016]
[CSO2016]	(Cantwell+Scaife+Oozeer+, 2016)
Write:	<<[CSO2016] JHHMMSS.ss+DDMMSS.ss>> <<[CSO2016] MACSJ2243.3-0935 A-N>>
N:	25+18
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	GMRT 610MHz observations of N=25+18 radio sources in the field of the merging cluster MACS J2243.3-0935.
in source:	MCS J2243.3-0935
Ref:	=2016MNRAS.458.1803C
by	CANTWELL T.M. , SCAIFE A.M.M., OOZEER N., WEN Z.L., HAN J.L.
	Mon. Not. R. Astron. Soc., 458, 1803-1814 (2016)
	A newly discovered radio halo in merging cluster MACS J2243.3-0935.
o	Table 4: <[CSO2016] JHHMMSS.ss+DDMMSS.ss> N=25. Table 5: <[CSO2016] MACSJ2243.3-0935 A-N> (Nos A-1 to A-9, B-1 to B-4, C-1 to C-5).
o	© 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CSOCA
CSOCA	(Catalog of Stars in Open Cluster Areas) (Not yet in Simbad)
Write:	<<CSOCA HH.hhhhhhhhh+DD.dddddddd>>
N:	171319
Object:	*inCl (SIMBAD class: Star)
Note:	Catalogue of stars in the [KPR2004b] 520 clusters
Ref:	=2004AN....325..740K
by	KHARCHENKO N.V. , PISKUNOV A.E., ROESER S., SCHILBACH E., SCHOLZ R.-D.
	Astron. Nachr., 325, 740-748 (2004)
	Astrophysical supplements to the ASCC-2.5. II. Membership probabilities in 520 Galactic open cluster sky areas.
o	Catalog: <CSOCA HH.hhhhhhhhh+DD.dddddddd> N=171319. Catalog: <[KPR2004b] NNN> (Nos 1-520).
=E=	Catalogue in electronic form as J/other/AN/325.740
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CSP2001]
[CSP2001]	(Clocchiatti+Suntzeff+Phillips+, 2001) (Not yet in Simbad)
Write:	<<[CSP2001] N>>
N:	7
Object:	* (SIMBAD class: Star)
Note:	N=7 refrence stars in the field of SN 1990B.
Ref:	=2001ApJ...553..886C
by	CLOCCHIATTI A. , SUNTZEFF N.B., PHILLIPS M.M., FILIPPENKO A.V., TURATTO M., BENETTI S., CAPPELLARO E., AVILES R., COVARRUBIAS R., DEGIOIA-EASTWOOD K., DICKINSON M., GOUIFFES C., GUHATHAKURTA P., HAMUY M., HEATHCOTE S.R., LEIBUNDGUT B., MATHESON T., NAVARRETE M., PEREZ M., PHILLIPS A., PIEMONTE A., RUIZ M.T., SHIELDS J.C., SMITH C., SPINRAD H., STURCH C.R., TYSON J.A., WELLS L.
	Astrophys. J., 553, 886-896 (2001)
	The type Ic SN 1990B in NGC 4568.
o	Fig.1: <[CSP2001] N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSP2004]
[CSP2004]	(Chand+Srianand+Petitjean+, 2004)
Write:	<<[CSP2004] QSO JHHMM+DDMM abs N.NNNN>>
N:	50
Object:	Absorber
Note:	Compilation of absorbers in the line of sight of 16 QSOs.
Ref:	=2004A&A...417..853C
by	CHAND H. , SRIANAND R., PETITJEAN P., ARACIL B.
	Astron. Astrophys., 417, 853-871 (2004)
	Probing the cosmological variation of the fine-structure constant: Results based on VLT-UVES sample.
o	Table 2: <[CSP2004] QSO JHHMM+DDMM abs N.NNNN> N=50.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSP2007]
[CSP2007]	(CHies-Santos+Santiago+Pastoriza, 2007)
Write:	<<[CSP2007] DD.ddddddd+DD.ddddddd>>
N:	187
Object:	GlCl (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Archival HST WFPC2 observations of NGC 1380.
Ref:	=2007A&A...467.1003C
by	CHIES-SANTOS A.L. , SANTIAGO B.X., PASTORIZA M.G.
	Astron. Astrophys., 467, 1003-1009 (2007)
	High resolution imaging of the early-type galaxy NGC 1380: an insight into the nature of extended extragalactic star clusters.
o	Catalog: <[CSP2007] DD.ddddddd+DD.ddddddd> N=187.
=E=	Catalogue in electronic form as J/A+A/467/1003
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSP2012]
[CSP2012]	(Castagne+Soucail+Pointecouteau+, 2012)
Write:	<<[CSP2012] NNN>>
N:	107
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	CFHT MOS spectroscopy of N=107 galaxies in Abell 1413.
in source:	ACO 1413
Ref:	=2012A&A...548A..18C
by	CASTAGNE D. , SOUCAIL G., POINTECOUTEAU E., CAPPI A., MAUROGORDATO S., BENOIST C., FERRARI C.
	Astron. Astrophys., 548A, 18-18 (2012)
	Deep optical observations of the massive galaxy cluster Abell 1413.
o	Table A.1: <[CSP2012] NNN> (Nos 1-107).
=E=	Catalogue in electronic form as <J/A+A/548/A18/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSP2015]
[CSP2015]	(Curtin+Shafter+Pritchet+, 2015)
Write:	<<[CSP2015] NNNNN YYYY-NNa>>
N:	27+37+19
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Stat:	is completely incorporated in Simbad
Note:	CFHT MegaCam observations of N=28+37+19 novae in three Virgo galaxies (NGC 4486, NGC 4472, and NGC 4374 respectively).
in source:	M 87 = Virgo A = NGC 4486
in source:	M 49 = NGC 4472
in source:	M 84 = NGC 4374
Ref:	=2015ApJ...811...34C
by	CURTIN C. , SHAFTER A.W., PRITCHET C.J., NEILL J.D., KUNDU A., MACCARONE T.J.
	Astrophys. J., 811, 34 (2015)
	Exploring the role of globular cluster specific frequency on the nova rates in three Virgo elliptical galaxies.
o	Tables 3-5: <[CSP2015] NNNNN YYYY-NNa> N=28+37+19.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSP2016]
[CSP2016]	(Carlin+Sand+Price+, 2016)= (MADCASH)
Write:	<<[CSP2016] MADCASH J074238+652501-dw>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Subaru Hyper Suprime-Cam (HSC) observation of N=1 dwarf galaxy companion of NGC 2403, as part of the Magellanic Analog Dwarf Companions And Stellar Halos (MADCASH) survey.
in source:	NGC 2403
Ref:	=2016ApJ...828L...5C
by	CARLIN J.L. , SAND D.J., PRICE P., WILLMAN B., KARUNAKARAN A., SPEKKENS K., BELL E.F., BRODIE J.P., CRNOJEVIC D., FORBES D.A., HARGIS J., KIRBY E., LUPTON R., PETER A.H.G., ROMANOWSKY A.J., STRADER J.
	Astrophys. J., 828L, 5-5 (2016)
	First results from the MADCASH survey: a faint dwarf galaxy companion to the low-mass spiral galaxy NGC 2403 at 3.2 Mpc.
o	Table 1: <MADCASH JHHMMSS+DDMMSS-dw> N=1 = <[CSP2016] MADCASH J074238+652501-dw> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
History	of this Acronym: replaced by MADCASH
Details on Acronym: [CSP85]
[CSP85]	(Couch+Shanks+Pence, 1985)
Write:	<<[CSP85] NNN>> <<[CSP85] AN>>
N:	171
Object:	G in ClG (SIMBAD class: Galaxy)
Note:	(Nos 1-171) in ClG 0055-279 (= CEMM J1888.16CL). Some 'NN' are also named '[AEC93] J1888.16CL NN' in 1993MNRAS.262..764A. (Nos A1-A4) are added in 1993MNRAS.262..764A and are also named '[AEC93] J1888.16CL AN'
in source:	ClG 0055-2754
Ref:	=1985MNRAS.213..215C
by	COUCH W.J. , SHANKS T., PENCE W.D.
	Mon. Not. R. Astron. Soc., 213, 215-241 (1985)
	CCD photometry of a cluster of galaxies at a redshift of 0.57.
o	<[CSP85] NNN> N=171
Ref:	=1993MNRAS.262..764A
by	ARAGON-SALAMANCA A. , ELLIS R.S., COUCH W.J., CARTER D.
	Mon. Not. R. Astron. Soc., 262, 764-794 (1993)
	Evidence for systematic evolution in the properties of galaxies in distant clusters.
o	Objects '[AEC93] J1888.16CL NN' = '[CSP85] NN', '[AEC93] J1888.16CL AN' = '[CSP85] AN', '[AEC93] 0016+16 NNN' = '[ECM85] NNN'.
o	Table 4: <[AEC93] HHMM+DD NNN>, <[AEC93] HHMM+DDMM NN>, <[AEC93] ANNNN.NNAA NNa> N=189. Table 4: <[AEC93] J1888.16CL AN> = <[CSP85] AN> (Nos A1-A4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSP94]
[CSP94]	(Collison+Saikia+Pedlar+, 1994)
Write:	<<[CSP94] NGC NNNN ANN>> <<[CSP94] NGC NNNN SS.ss+SS.s>>
N:	14+11+1+2+1+3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 1: format 'NGC NNNN AN', where 'AN' stands for radio-components of galaxies Table 2: format 'NGC NNNN SS.ss-SS.s', cross-identified with the format in table 1.
in source:	NGC 253
in source:	NGC 1808
in source:	NGC 2146
in source:	NGC 2633
in source:	NGC 2782
in source:	NGC 4321
Ref:	=1994MNRAS.268..203C
by	COLLISON P.M. , SAIKIA D.J., PEDLAR A., AXON D.J., UNGER S.W.
	Mon. Not. R. Astron. Soc., 268, 203-212 (1994)
	Radio continuum observations of starburst galaxies.
o	Table 1: <[CSP94] NGC NNNN ANN> N=14+11+1+2+1+3. Table 2: <[CSP94] NGC NNNN SS.ss-SS.s> N14+11+1+2+1+3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSR2005]
[CSR2005]	(Comeron+Schneider+Russeil, 2005)
Write:	<<[CSR2005] Star NN>> <<[CSR2005] Star NNA>>
N:	25+18
Object:	* (SIMBAD class: Star)
Note:	ESO NTT NIR observations. N=25 stars projected on the HII region IRAS 16362-4845 in the western part of RCW 108. N=7 of the stars are multiple systems with a format NNA. See also [CS2007].
in source:	RCW 108
Ref:	=2005A&A...433..955C
by	COMERON F. , SCHNEIDER N., RUSSEIL D.
	Astron. Astrophys., 433, 955-977 (2005)
	Star formation in RCW 108: Triggered or spontaneous?
o	paragr. 6.1: IRAS 16362-4849 is a misprint for IRAS 16362-4845.
o	Table 2: <[CSR2005] Star NN> (Nos 1-25).
Ref:	=2007A&A...473..149C
by	COMERON F. , SCHNEIDER N.
	Astron. Astrophys., 473, 149-162 (2007)
	A close look at the heart of RCW 108.
o	Table 2: <[CS2007] NNN> (Nos 1-147). Table 2: <[CSR2005] Star NNA> N=18.
=E=	Catalogue in electronic form as J/A+A/473/149
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSR2018]
[CSR2018]	(Cava A.+Schaerer D.+Richard+, 2018)
Write:	<<[CSR2018] Cosmic Snake>> <<[CSR2018] Counterimage>> <<[CSR2018] Source Galaxy>> <<[CSR2018] MACS J1206.2-0847 A.N>> <<[CSR2018] MACS J1206.2-0847 GN>> <<[CSR2018] MACS J1206.2-0847 BCG>>
N:	1+1+16+1+4+1
Object:	Grav. lensed image of a G + G + G in ClG + Brightest Cluster Galaxy (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=1+1+16 gravitationally lensed images of N=1 background galaxy, lensed by the galaxy cluster MCS J1206.2-0847. N=4 cluster members and N=1 brightest cluster galaxy (BCG). Use of HST CLASH data.
Ref:	=2018NatAs...2...76C
by	CAVA A. , SCHAERER D., RICHARD J., PEREZ-GONZALEZ P.G., DESSAUGES-ZAVADSKY M., MAYER L., TAMBURELLO V.
	NatAs, 2, 76-82 (2018)
	The nature of giant clumps in distant galaxies probed by the anatomy of the Cosmic Snake.
o	<[CSR2018] Cosmic Snake> N=1. <[CSR2018] Counterimage> N=1. <[CSR2018] Source Galaxy> N=1. Fig. 8, Table 4: <[CSR2018] MACS J1206.2-0847 A.N> N=16. Fig. 8, Table 5: <[CSR2018] MACS J1206.2-0847 GN> (Nos G1-G4), <[CSR2018] MACS J1206.2-0847 BCG> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSR96]
[CSR96]	(Claeskens+Surdej+Remy, 1996)
Write:	<<[CSR96] J03.13 A>>
N:	2
Object:	Component of QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	N=2 point-like components of CTS J03.13
in source:	CTS J03.13
Ref:	=1996A&A...305L...9C
by	CLAESKENS J.-F. , SURDEJ J., REMY M.
	Astron. Astrophys., 305, 9-12 (1996)
	J03.13 A and B: a new multiply imaged QSO candidate.
o	J03.13 = CTS 286
o	Table 3: <[CSR96] J03.13 A> (Nos A-B)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSR98]
[CSR98]	(Canalizo+Stockton +Roth, 1998)
Write:	<<[CSR98] HHMM+DDMM>>
N:	1
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Ref:	=1998AJ....115..890C
by	CANALIZO G. , STOCKTON A., ROTH K.C.
	Astron. J., 115, 890-894 (1998)
	Serendipitous discovery of a broad absorption line QSO at z = 2.169.
o	<[CSR98] 0134+3253> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CSRG
CSRG	(Catalog of Southern Ringed Galaxies)
Write:	<<CSRG NNNN>>
N:	1235
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Table 3, col. (2)
Ref:	=1995ApJS...96...39B
by	BUTA R.
	Astrophys. J., Suppl. Ser., 96, 39-116 (1995)
	The catalog of southern ringed galaxies.
o	(Erratum) Erratum 1995 ApJS 98, p. 739
o	Table 3, col.(2): <CSRG NNNN> N=1235, Table 6, col.(2): <ACSRG NNN> N=175.
=E=	Catalogue in electronic form as J/ApJS/96/39
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CSS
CSS	(Catalina Sky Survey)
*****	Avoid the usage of CSS, prefer CRTS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CSS
CSS	(Catalog of S *)= (CGSS) = (CSS1)
Write:	<<CSS NNNN>>
N:	1347
Object:	S * (SIMBAD class: Star)
Note:	Compilation on galactic S stars, superseding 1976PW&SO...2....2S. No maps. Table 1: (Nos 1-1347), general catalogue of S stars. Table 2: objects not numbered, stars that have been published as S stars but probably or definitely are not.
Ref:	=1984PW&SO...3....1S
by	STEPHENSON C.B.
	Publ. Warner & Swasey Obs., 3, 1-49 (1984)
	A General Catalog of S Stars, second edition.
o	Table 1: <CSS NNNN> (Nos 1-1347)
=E=	Catalogue in electronic form as III/168
Details on Acronym: CSS
CSS	(Carpenter+Snell+Schloerb)
*****	Avoid the usage of CSS, prefer [CSS95]
Origin	of the Acronym: L (2003A&A...397..177B)
Details on Acronym: CSS
CSS	(Catalina Sky Survey)
*****	Avoid the usage of CSS, prefer [DDM2009]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CSS
CSS	(Compact Steep-Spectrum source)
*****	Avoid the usage of CSS, prefer [TSR2003]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CSS1
CSS1	(Catalog of S *, list 1)
*****	Avoid the usage of CSS1, prefer CSS
Details on Acronym: CSS2
CSS2	(Catalog of S *, list 2)
Write:	<<CSS2 NN>>
N:	75
Object:	S * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Complement to the catalog CSS
Ref:	=1990AJ....100..569S
by	STEPHENSON C.B.
	Astron. J., 100, 569-571 (1990)
	New and relatively faint S stars found in the Northern Milky Way.
o	Table I: <CSS2 NN> (Nos 1-75)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSS2000]
[CSS2000]	(Chapman+Scott+Steidel+, 2000)= (H)
Write:	<<[CSS2000] ANN>> <<[CSS2000] AANN>>
N:	5+8
Object:	G (SIMBAD class: Galaxy)
Note:	SCUBA observations of galaxies in HDF flanking fields.
in source:	NAME HDFN
Ref:	=2000MNRAS.319..318C
by	CHAPMAN S.C. , SCOTT D., STEIDEL C.C., BORYS C., HALPERN M., MORRIS S.L., ADELBERGER K.L., DICKINSON M., GIAVALISCO M., PETTINI M.
	Mon. Not. R. Astron. Soc., 319, 318-330 (2000)
	A search for the submillimetre counterparts to Lyman break galaxies.
o	Table 1: <Westphal AANN> (Nos CC1, CC76, DD20, MM8, MM27), <Westphal AAANNN> (Nos MMD11, MMD46, MMD109). Tables 1, 2: <[CSS2000] ANN> (Nos C10, C38, D2), <[CSS2000] AANN> (Nos MM17, MM18). Table 2: <[SAD98] 22a AANN> (Nos MD6, MD55, M17), <[SAD98] 22b AANN> (No. MD36).
Ref:	=2001ApJ...562...95S
by	SHAPLEY A.E. , STEIDEL C.C., ADELBERGER K.L., DICKINSON M., GIAVALISCO M., PETTINI M.
	Astrophys. J., 562, 95-123 (2001)
	The rest-frame optical properties of z≃3 galaxies.
o	Table 3: <[SSA2001] HDF oAANN> (Nos oC37, oC38, oMD49, oM5), <[SSA2001] DSF2237a AANN> N=18, <[SSA2001] Westphal west3 C11> N=1, <[SSA2001] SSA22a aug96 D1> N=1, <[SSA2001] SSA22b oct96 D8> N=1. Table 3: <[CSS2000] AANN> (Nos CC24, DD3, DD15) and N=5 among (Nos MM7 to MM28) added. Table 3: <[PKS98] QHHMM+DDd> AAANN> N=7 added, <[PKS98] B2 0902+343 AANN> N=9 added, <[PKS98] 3C 324 ANN>, <[PKS98] 3C 324 AAN> N=2 added. Table 3: <[PSS2001] CDFa AANN> N=5 added. Table 3: <[SAD98] SSA 22a AANN> N=19+1 added. Table 3: <Westphal AAANNN> N=23 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSS2002]
[CSS2002]	(Chapman+Shapley+Steidel+, 2002) (Not yet in Simbad)
Write:	<<[CSS2002] BN>> <<[CSS2002] RN>>
N:	3
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Note:	N=2 Blue (Nos B1-B2) and N=1 Red (Nos R3) components of the galaxy Westphal MMD11.
in source:	Westphal MMD11
Ref:	=2002ApJ...572L...1C
by	CHAPMAN S.C. , SHAPLEY A., STEIDEL C., WINDHORST R.
	Astrophys. J., 572, 1-5 (2002)
	Westphal-MMD 11: an interacting, submillimeter luminous Lyman break galaxy.
o	Parag. 3 : IRAS 22491 = IRAS 22491-1808 (= PGC 69877)
o	Fig.1: <[CSS2002] AN> (Nos B1, B2, R3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSS2003]
[CSS2003]	(Cotton+Spencer+Saikia+, 2003) (Not yet in Simbad)
Write:	<<[CSS2003] 3C 43 A>> <<[CSS2003] 3C 454 A>>
N:	8+4
Object:	(Rad) component (SIMBAD class: Radio = Radio Source)
Note:	VLA, MERLIN and VLBA components at 18 cm of 3C 43 and 3C 454.
in source:	3C 43
in source:	3C 454
Ref:	=2003A&A...403..537C
by	COTTON W.D. , SPENCER R.E., SAIKIA D.J., GARRINGTON S.
	Astron. Astrophys., 403, 537-546 (2003)
	Faraday rotation in the CSS QSOs 3C 43 and 3C 454.
o	Figs 1, 6, Table 1: <[CSS2003] 3C 43 A> (Nos A-H), <[CSS2003] 3C 454 A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSS2004]
[CSS2004]	(Chen+Su+Slane+, 2004)
Write:	<<[CSS2004] NN>>
N:	52
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-S observations of 3C 391 field.
Ref:	=2004ApJ...616..885C
by	CHEN Y. , SU Y., SLANE P.O., WANG Q.D.
	Astrophys. J., 616, 885-894 (2004)
	A Chandra ACIS view of the thermal composite supernova remnant 3C 391.
o	Regions in Table 2 and Fig.1(d) are not in SIMBAD.
o	Table 1: <[CSS2004] NN> (Nos 1-52).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSS2005]
[CSS2005]	(Christopher+Scoville+Stolovy+, 2005) (Not yet in Simbad)
Write:	<<[CSS2005] Core A>> <<[CSS2005] Core AA>>
N:	27
Object:	Core (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	OVRO mm array observations of HCN in the Galactic Center.
in source:	NAME Gal Center
Ref:	=2005ApJ...622..346C
by	CHRISTOPHER M.H. , SCOVILLE N.Z., STOLOVY S.R., YUN M.S.
	Astrophys. J., 622, 346-365 (2005)
	HCN and HCO^+ observations of the galactic circumnuclear disk.
o	Table 2, Fig.13: <[CSS2005] Core A> (Nos A-Z).
Ref:	=2008ApJ...683L.147Y
by	YUSEF-ZADEH F. , BRAATZ J., WARDLE M., ROBERTS D.
	Astrophys. J., 683L, 147-150 (2008)
	Massive star formation in the molecular ring orbiting the black hole at the galactic center.
o	Text: <[CSS2005] Core AA> (No. AA) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSS2008]
[CSS2008]	(Chen+Seward+Sun+, 2008)
Write:	<<[CSS2008] NN>>
N:	30
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of Kes 27.
in source:	Kes 27
Ref:	=2008ApJ...676.1040C
by	CHEN Y. , SEWARD F.D., SUN M., LI J.-T.
	Astrophys. J., 676, 1040-1049 (2008)
	The thermal composite supernova remnant Kesteven 27 as viewed by Chandra: shock reflection from a cavity wall.
o	Table 1: <[CSS2008] NN> (Nos 1-30).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSS2011]
[CSS2011]	(Clayton+Sugerman+Stanford+, 2011) (Not yet in Simbad)
Write:	<<[CSS2011] N>>
N:	6
Object:	Cometary Globule (SIMBAD class: ComGlob = Cometary Globule / Pillar)
Note:	Gemini South GMOS, HST WFPC2, Spitzer MIPS and Herschel SPIRE observations of N=6 cometary globules around R Coronae Borealis.
Ref:	=2011ApJ...743...44C
by	CLAYTON G.C. , SUGERMAN B.E.K., STANFORD S.A., WHITNEY B.A., HONOR J., BABLER B., BARLOW M.J., GORDON K.D., ANDREWS J.E., GEBALLE T.R., BOND H.E., DE MARCO O., LAWSON W.A., SIBTHORPE B., OLOFSSON G., POLEHAMPTON E., GOMEZ H.L., MATSUURA M., HARGRAVE P.C., IVISON R.J., WESSON R., LEEKS S.J., SWINYARD B.M., LIM T.L.
	Astrophys. J., 743, 44 (2011)
	The circumstellar environment of R Coronae Borealis: white dwarf merger or final-helium-shell flash?
o	Fig. 4: <[CSS2011] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSS2016]
[CSS2016]	(Costa+Spangler+Sink+, 2016)= ([CSS2016a])
Write:	<<[CSS2016] NNN>>
N:	10
Object:	Rad (SIMBAD class: Radio = Radio Source)
Note:	NRAO VLA observations of N=7 extragalactic radio sources with lines of sight through the Rosette Nebula.
Ref:	=2016ApJ...821...92C
by	COSTA A.H. , SPANGLER S.R., SINK J.R., BROWN S., MAO S.A.
	Astrophys. J., 821, 92-92 (2016)
	Denser sampling of the rosette nebula with Faraday rotation measurements: improved estimates of magnetic fields in H II regions.
o	Table 2: <[SSF2013] INN> (Nos I9, I11, I13, I17) added. Table2: <[CSS2016] NNN> (Nos N4-N10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSS2016a]
[CSS2016a]	(Costa+Spangler+Sink+, 2016)
*****	Avoid the usage of [CSS2016a], prefer [CSS2016]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSS2016b]
[CSS2016b]	(Crnojevic+Sand+Spekkens+, 2016) (Not yet in Simbad)
Write:	<<[CSS2016b] Cloud S>>
Object:	Stellar Density (SIMBAD class: Stream = Stellar Stream)
Note:	Magellan Clay telescope Megacam observations of N=1 stellar density to the south of Centaurus A.
in source:	Cen A = NGC 5128
Ref:	=2016ApJ...823...19C
by	CRNOJEVIC D. , SAND D.J., SPEKKENS K., CALDWELL N., GUHATHAKURTA P., McLEOD B., SETH A., SIMON J.D., STRADER J., TOLOBA E.
	Astrophys. J., 823, 19-19 (2016)
	The extended halo of Centaurus A: uncovering satellites, streams, and substructures.
o	Fig. 4, Tables 1+3: <[CSC2014] CenA-MM-DwN> (Nos Dw3-Dw13). Fig. 4, Paragr. 4.4: <[CSS2016b] Cloud S> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSS2017]
[CSS2017]	(Caldwell+Strader+Sand+, 2017) (Not yet in Simbad)
Write:	<<[CSS2017] And I-GC1>>
N:	1
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	N=1 globular cluster in the dwarf galaxy And I. Use of HST archival data.
in source:	And I
Ref:	=2017PASA...34...39C
by	CALDWELL N. , STRADER J., SAND D.J., WILLMAN B., SETH A.C.
	PASA, 34, 39 (2017)
	The faint globular cluster in the dwarf galaxy Andromeda I.
o	<[CSS2017] And I-GC1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSS91]
[CSS91]	(Cappellaro+Sabbadin+Salvadori+, 1991)
Write:	<<[CSS91] HHMMSS+DDMM>>
N:	1
Object:	G (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Fig.5: N=1 emission-line galaxy. The 2 PN in Figs 1 and 3 are CSST.
Ref:	=1991Msngr..64...39C
by	CAPPELLARO E. , SABBADIN F., SALVADORI L., TURATTO M.
	The Messenger, 64, 39-None (1991)
	New distant planetary nebulae.
o	Figs 1, 3: <CSST N> (Nos 1-2). Fig.5: <[CSS91] HHMMSS+DDMM> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSS93]
[CSS93]	(Carpenter J.M.+Snell R.L.+Schloerb F.P.+, 1993) (Not yet in Simbad)
Write:	<<[CSS93] IRAS HHMMm+DDMM Cluster>> <<[CSS93] IRAS HHMMm+DDMM Core>>
Object:	Cluster of * + CS Core (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Wyoming Infrared Observatory (WIRO) 2.3m telescope NIR and FCRAO 14m telescope CS(2-1)observations of N=17 star clusters and N=20 dense cores associated with 20 IRAS sources.
Ref:	=1993ApJ...407..657C
by	CARPENTER J.M. , SNELL R.L., SCHLOERB F.P., SKRUTSKIE M.F.
	Astrophys. J., 407, 657-679 (1993)
	Embedded star clusters associated with luminous IRAS point sources.
o	Table 2: <[CSS93] IRAS HHMMm+DDMM Cluster> N=17, <[CSS93] IRAS HHMMm+DDMM Core> N=20.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSS95]
[CSS95]	(Carpenter+Snell+Schloerb, 1995)= (CSS) = (Gem)
Write:	<<[CSS95] core NN>> <<[CSS95] Cl Na>>
N:	16+6
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Table 2: format 'core NN', N=16 dense cores Table 4: format 'Cl Na', N=6 Cl*, (Nos 1a, 1b, 2, 3, 4a, 4b) Table 1: 2 regions added from the ref. 1995ApJ...445..246C, but regions of observation, not objects
in source:	NAME ASS GEM OB 1-
Ref:	=1995ApJ...450..201C
by	CARPENTER J.M. , SNELL R.L., SCHLOERB F.P.
	Astrophys. J., 450, 201-216 (1995)
	Star formation in the Gemini OB1 molecular cloud complex.
o	Table 1: regions of observation, not in SIMBAD
o	Table 2: <[CSS95] core NN> (Nos 1-16), Table 3: <[CSS95] Cl Na> (Nos 1a, 1b, 2, 3, 4a, 4b)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CSST
CSST	(Cappellaro+Sabbadin+Salvadori+Turatto)
Write:	<<CSST N>>
N:	2
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Figs 1 and 3: N=2 PN, CSST 1 and 2. Fig.5: N=1 emission-line galaxy, [CSS91].
Ref:	=1991Msngr..64...39C
by	CAPPELLARO E. , SABBADIN F., SALVADORI L., TURATTO M.
	The Messenger, 64, 39-None (1991)
	New distant planetary nebulae.
o	Figs 1, 3: <CSST N> (Nos 1-2). Fig.5: <[CSS91] HHMMSS+DDMM> N=1.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CST2016]
[CST2016]	(Cowley+Spitler+Tran+, 2016)
Write:	<<[CST2016] NNN>>
N:	235
Object:	Poss. AGN (SIMBAD class: AGN_Candidate = Active Galaxy Nucleus Candidate)
Note:	Magellan Baade 6.5m telescope NIR photometric observations of N=235 active galactic nuclei (AGN) candidates in the CDFS, COSMOS and UDS fields as part of the FourStar Galaxy Evolution (zFourGE) survey. Use of archival Spitzer IRAC and HST CANDELS data. See also [SLG2012], [TPT2013] and [SLS2014].
Ref:	=2016MNRAS.457..629C
by	COWLEY M.J. , SPITLER L.R., TRAN K.-V.H., REES G.A., LABBE I., ALLEN R.J., BRAMMER G.B., GLAZEBROOK K., HOPKINS A.M., JUNEAU S., KACPRZAK G.G., MULLANEY J.R., NANAYAKKARA T., PAPOVICH C., QUADRI R.F., STRAATMAN C.M.S., TOMCZAK A.R., VAN DOKKUM P.G.
	Mon. Not. R. Astron. Soc., 457, 629-641 (2016)
	ZFOURGE catalogue of AGN candidates: an enhancement of 160-µm-derived star formation rates in active galaxies to z = 3.2.
o	Table A.1: <[CST2016] NNN> (Nos 1-235).
=E=	Catalogue in electronic form as <J/MNRAS/457/629/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CST94]
[CST94]	(Chengalur+Salpeter+Terzian, 1994)
Write:	<<[CST94] A>>
N:	6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Ref:	=1994AJ....107.1984C
by	CHENGALUR J.N. , SALPETER E.E., TERZIAN Y.
	Astron. J., 107, 1984-2005 (1994)
	Dynamics of binary galaxies. II. Close pairs.
o	Table 3: <[CST94] A> (Nos A-F) N=6
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CSTAR
CSTAR	(Chinese Small Telescope ARray) (Not yet in Simbad)
*****	Avoid the usage of CSTAR, prefer [OMW2016]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CSTAR
CSTAR	(Chinese Small Telescope ARray) (Not yet in Simbad)
*****	Avoid the usage of CSTAR, prefer [WMW2013]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CSTAR
CSTAR	(Chinese Small Telescope ARray)
*****	Avoid the usage of CSTAR, prefer [WMK2011]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CStars
CStars	(Carbon *)
====>	Equivalent to: C*
Details on Acronym: CSV
CSV	(Catalog of Suspected Variable *)= (K) = (KZP)
Write:	<<CSV NNNNNNA>>
N:	12000
Object:	Susp. V* (SIMBAD class: Variable* = Variable Star)
Note:	1st ref.: N=8000. 2nd ref.: N=4000. There are doubtful cases in both refs. Updated and superseded by NSV.
Ref:	=1951CSV...C......0K
by	KUKARKIN B.V. , PARENAGO P.P., EFREMOV Y.N., KHOLOPOV P.N.
	Moscow, Acad. of Sciences USSR Shternberg,1951, 0-None (1951)
	Catalogue of suspected variable stars.
o	<CSV NNNNNNA> (Nos 1-5835, 100000-102299).
Ref:	=1965CSV...C......0K
by	KUKARKIN B.V. , KHOLOPOV P.N., EFREMOV Y.N., KUROCHKIN N.E.
	Moscow, Acad. of Sciences USSR Shternberg,1951, 0-None (1965)
	Second catalogue of suspected variable stars.
o	<CSV NNNNNNA> (Nos 5836-9877, 102300-103137).
Details on Acronym: [CSV2005]
[CSV2005]	(Colbert+Strickland+Veilleux+, 2005)
Write:	<<[CSV2005] NN>>
N:	20
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS observations of NGC 2992.
in source:	NGC 2992
Ref:	=2005ApJ...628..113C
by	COLBERT E.J.M. , STRICKLAND D.K., VEILLEUX S., WEAVER K.A.
	Astrophys. J., 628, 113-128 (2005)
	Extranuclear X-ray emission in the edge-on Seyfert galaxy NGC 2992.
o	Table 1: <[CSV2005] NN> (Nos 1-20).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSV2006]
[CSV2006]	(Cox+Sparke+Van Moorsel, 2006)
Write:	<<[CSV2006] N>>
N:	5
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLA HI observations of UGC 9796: 5 galaxy companions are found.
Ref:	=2006AJ....131..828C
by	COX A.L. , SPARKE L.S., VAN MOORSEL G.
	Astron. J., 131, 828-836 (2006)
	Neutral hydrogen in the polar ring galaxy UGC 9796.
o	Table 2: <[CSV2006] N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSV96]
[CSV96]	(Churchill+Steidel+Vogt, 1996)
Write:	<<[CSV96] GNN>>
N:	15
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Ref:	=1996ApJ...471..164C
by	CHURCHILL C.W. , STEIDEL C.C., VOGT S.S.
	Astrophys. J., 471, 164-172 (1996)
	On the spatial and kinematic distributions of Mg II absorbing gas in < z> ~ 0.7 galaxies.
o	Table 2: <[CSV96] GNN> (Nos G1-G15)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSW2004]
[CSW2004]	(Chapman+Scott+Windhorst+, 2004)
Write:	<<[CSW2004] JN>> <<[CSW2004] JHHMMSS.sss+DDMMSS.ss>>
N:	4+1
Object:	(X) + (Rad) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	In the HST image of [SAS2000] Blob 1 4 sources JN are found (J1 to J4) In the SCUBA map of [SAS2000] Blob 1, a radio source is identified.
Ref:	=2004ApJ...606...85C
by	CHAPMAN S.C. , SCOTT D., WINDHORST R.A., FRAYER D.T., BORYS C., LEWIS G.F., IVISON R.J.
	Astrophys. J., 606, 85-91 (2004)
	Further multiwavelength observations of the SSA 22 Lyα-emitting blob.
o	In the introduction SMM J16034 (2003MNRAS.342.1185) is probably SMM J163650.0+405733 ([CBI2003] SMM J163650.0+405733 in SIMBAD).
o	Fig.1: <[CSW2004] AN> (Nos J1-J4). Fig.5: <[CSW2004] JHHMMSS.sss+DDMMSS.ss> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CSW2006]
[CSW2006]	(Cannon+Smith+Walter+, 2006)
Write:	<<[CSW2006] DN>>
N:	2
Object:	Region (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC and MIPS observations of NGC 1705: Dust emission regions are found.
in source:	NGC 1705
Ref:	=2006ApJ...647..293C
by	CANNON J.M. , SMITH J.-D.T., WALTER F., BENDO G.J., CALZETTI D., DALE D.A., DRAINE B.T., ENGELBRACHT C.W., GORDON K.D., HELOU G., KENNICUTT R.C.Jr, LEITHERER C., ARMUS L., BUCKALEW B.A., HOLLENBACH D.J., JARRETT T.H., LI A., MEYER M.J., MURPHY E.J., REGAN M.W., RIEKE G.H., RIEKE M.J., ROUSSEL H., SHETH K., THORNLEY M.D.
	Astrophys. J., 647, 293-302 (2006)
	Warm dust and spatially variable polycyclic aromatic hydrocarbon emission in the dwarf starburst galaxy NGC 1705.
o	Table 1, Fig.1: <[CSW2006] DN> (Nos D1-D2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CSWA
CSWA	(Cambridge Sloan Survey of Wide Arcs)= (CASSOWARY)
Write:	<<CSWA NNN>> <<CSWA NNN.N>>
Object:	Grav. lens system (SIMBAD class: GravLensSystem = Gravitational Lens System (lens+images))
Note:	Sytematic search for wide-separation gravitational lens systems, looking for multiple, blue companions around massive ellipticals in the SDSS photometric catalogue. The updated catalogue is available at http://www.ast.cam.ac.uk/research/cassowary/
Ref:	=2009MNRAS.392..104B
by	BELOKUROV V. , EVANS N.W., HEWETT P.C., MOISEEV A., McMAHON R.G., SANCHEZ S.F., KING L.J.
	Mon. Not. R. Astron. Soc., 392, 104-112 (2009)
	Two new large-separation gravitational lenses from SDSS.
o	Fig. 1, Tables 1-2: <CSWA NN> N=7 among (Nos 1-13). Fig.4, Table 2: <[BEH2009] CSWA 2 LN> (Nos L1-L2), <[BEH2009] CSWA 2 A> (Nos A-G). Fig. 4, Table 3: <[BEH2009] CSWA 3 L>, <[BEH2009] CSWA 3 A> (Nos A-C).
Ref:	=2010MNRAS.402.2335P
by	PETTINI M. , CHRISTENSEN L., D'ODORICO S., BELOKUROV V., EVANS N.W., HEWETT P.C., KOPOSOV S., MASON E., VERNET J.
	Mon. Not. R. Astron. Soc., 402, 2335-2343 (2010)
	CASSOWARY20: a wide separation EINSTEIN cross identified with the X-shooter spectrograph.
o	<CSWA NN> (No. 20) added. Fig. 1, Table 1: <[PCD2010] Lens> N=1, <[PCD2010] iN> (Nos i1-i4).
Ref:	=2010MNRAS.406.2616C
by	CHRISTENSEN L. , D'ODORICO S., PETTINI M., BELOKUROV V., EVANS N.W., KELLOGG M., VERNET J.
	Mon. Not. R. Astron. Soc., 406, 2616-2626 (2010)
	X-shooter observations of the gravitational lens system CASSOWARY 5.
o	<CSWA NN> (No. 5). Fig. 1, Table 1: <[CDP2010] LN> (Nos L1-L2), <[CDP2010] imN> (Nos im1-im4).
Ref:	=2013MNRAS.436.1040S
by	STARK D.P. , AUGER M., BELOKUROV V., JONES T., ROBERTSON B., ELLIS R.S., SAND D.J., MOISEEV A., EAGLE W., MYERS T.
	Mon. Not. R. Astron. Soc., 436, 1040-1056 (2013)
	The CASSOWARY spectroscopy survey: a new sample of gravitationally lensed galaxies in SDSS.
o	Tables 1+2+4: <[SAB2013] SDSS JHHMM+DDMM> N=28, <[SAB2013] SDSS JHHMM+DDMM lens> N=28, <[SAB2013] SDSS JHHMM+DDMM source> N=29, <[SAB2013] SDSS JHHMM+DDMM source a> N=4. Table 3: <[SAB2013] SDSS JHHMM+DDMM cont> N=6. Table 4, col(2): <CSWA NNN> N=51 among (Nos 1-165).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CT
CT	(Choi+Tatematsu)
*****	Avoid the usage of CT, prefer [CT2004]
Origin	of the Acronym: L (2008ApJ...687..406C)
Details on Acronym: CT
CT	(Campusano+Torres)
*****	Avoid the usage of CT, prefer [CT83]
Details on Acronym: CT
CT	(Calan Tololo survey)
*****	Avoid the usage of CT, prefer CTS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CT
CT	(Coma, Tifft)
*****	Avoid the usage of CT, prefer [TG73]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CT2004]
[CT2004]	(Choi+Tatematsu, 2004)= (CT)
Write:	<<[CT2004] N>>
N:	5
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA observations. N=5 millimeter continuum sources in the R CrA [TS84] IRS 7 region.
in source:	NAME R CrA Cloud
Ref:	=2004ApJ...600L..55C
by	CHOI M. , TATEMATSU K.
	Astrophys. J., 600, 55-58 (2004)
	High-resolution millimeter imaging of the R Coronae Australis IRS 7 region.
o	R CrA IRS 7 = [TS84] IRS 7 in SIMBAD
o	Fig.1, Table 1: <[CT2004] N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CT2008]
[CT2008]	(Chen+Tinker, 2008)
Write:	<<[CT2008] HHMM+DDMM N.NNNN>> <<[CT2008] 3C 336 N.NNNNa>> <<[CT2008] QSO JHHMM+DDMM abs N.NNNN>>
N:	11+13+13
Object:	G + ALS (SIMBAD class: Galaxy)
Note:	Magellan Clay telescope MIKE echelle spectrograph observations of Galaxy-MgII absorber pairs in the field of N=7 QSOs.
Ref:	=2008ApJ...687..745C
by	CHEN H.-W. , TINKER J.L.
	Astrophys. J., 687, 745-756 (2008)
	The baryon content of dark matter halos: empirical constraints from Mg II absorbers.
o	Table 2, col(z(gal)): <[CT2008] HHMM+DDMM N.NNNN> N=11, Table 2, col(z(gal)): <[CT2008] 3C 336 N.NNNNa> N=13. Table 2, col(z(abs)): <[CT2008] QSO JHHMM+DDMM abs N.NNNN> N=13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 4CT
4CT	(4th Cambridge catalog, Total flux)= 4C(T)
Write:	<<4CT DD.NN.NA>> <<4CT +DD.NN>>
N:	86
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	1st ref.: N=86 new sources not in the 4C catalogue. 2nd ref.: The source 64.20.1 is divided into 3 components A to C
Ref:	=1969MNRAS.145..181C
by	CASWELL J.L. , CROWTHER J.H.
	Mon. Not. R. Astron. Soc., 145, 181-196 (1969)
	A pencil-beam survey of radio sources at 178 MHz.
o	Table II: <4CT DD.NN.N> N=86
Ref:	=1974MNRAS.166..101S
by	SLINGO A.
	Mon. Not. R. Astron. Soc., 166, 101-111 (1974)
	Observations of ten extragalactic radio sources with very steep spectra.
o	Table I: <[S74] 64.20.1 A> (Nos A-C).
Details on Acronym: [CT83]
[CT83]	(Campusano+Torres, 1983)= (CT) = ([CT83a])
Write:	<<[CT83] NNN>>
N:	373
Object:	UV Exc. Obj. (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	Identif. charts
Ref:	=1983AJ.....88.1304C
by	CAMPUSANO L.E. , TORRES C.
	Astron. J., 88, 1304-1322 (1983)
	The Cerro el Roble sample of faint ultraviolet excess objects in the South Galactic Pole.
o	Table II: <[CT83] NNN> (Nos 1-373)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CT83a]
[CT83a]	(Campusano+Torres, 1983)
*****	Avoid the usage of [CT83a], prefer [CT83]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CT83b]
[CT83b]	(Christian+Tully, 1983)
Write:	<<[CT83b] NN>>
N:	66
Object:	* (SIMBAD class: Star)
in source:	LGS 3
Ref:	=1983AJ.....88..934C
by	CHRISTIAN C.A. , TULLY B.R.
	Astron. J., 88, 934-938 (1983)
	The local group irregular galaxies LGS 3 and Pegasus.
o	<[CT83b] NN> (Nos 1-66)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CT96]
[CT96]	(Crotts+Tomaney, 1996)
Write:	<<[CT96] JHHMMSS.s+DDMMSS>>
N:	6
Object:	Poss. Microlensing Event (SIMBAD class: LensingEv = (Micro)Lensing Event)
Stat:	is completely incorporated in Simbad
in source:	M 31 = NGC 224
Ref:	=1996ApJ...473L..87C
by	CROTTS A.P.S. , TOMANEY A.B.
	Astrophys. J., 473, 87-90 (1996)
	Results from a survey of gravitational microlensing toward M31.
o	Table 1: <[CT96] JHHMMSS.s+DDMMSS> N=6
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CTA
CTA	(Caltech obs., list A)
Write:	<<CTA NNN>>
N:	106
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1960PASP...72..237H
by	HARRIS D.E. , ROBERTS J.A.
	Publ. Astron. Soc. Pac., 72, 237-255 (1960)
	Radio source measurements at 960 MC/S.
o	Table I: <CTA NNN> (Nos 1-106)
Details on Acronym: CTB
CTB	(Caltech obs., list B)= (WB)
Write:	<<CTB NNNa>> <<CTB NNNA>> (not recognised by Simbad, but found in literature)
N:	110+8
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Discrete radio sources in the galactic plane.
Ref:	=1960PASP...72..331W
by	WILSON R.W. , BOLTON J.G.
	Publ. Astron. Soc. Pac., 72, 331-347 (1960)
	A survey of galactic radiation at 960 MC/S.
o	<CTB NNN> (Nos 1-110)
Ref:	=1963AJ.....68..181W
by	WILSON R.W.
	Astron. J., 68, 181-185 (1963)
	Catalogue of radio sources in the Galactic plane.
o	Table I: <CTB NNNa> (Nos 90a-90b, 91a-91b, 104a-104b) added.
Ref:	=1978ApJS...38..119V
by	VAN DEN BERGH S.
	Astrophys. J., Suppl. Ser., 38, 119-128 (1978)
	A systematic search for galactic Supernova Remnants.
o	Fig.8: <PN VBe N> (No. 1). Table 1: <CTB NNNa> (Nos 37a, 37b).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CTB2011]
[CTB2011]	(Croft+Tomsick+Bower, 2011)
Write:	<<[CTB2011] XNNN>>
N:	128
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra X-ray observations of steady or transient VLA radio sources.
Ref:	=2011ApJ...740...87C
by	CROFT S. , TOMSICK J.A., BOWER G.C.
	Astrophys. J., 740, 87 (2011)
	X-ray observations of radio transients without optical hosts.
o	Table 2: <[CTB2011] XNNN> (Nos X1-X128).
=E=	Catalogue in electronic form as J/ApJ/740/87
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTB2016]
[CTB2016]	(Consiglio+Turner+Beck+, 2016)
Write:	<<[CTB2016] Cloud W>> <<[CTB2016] Cloud C>> <<[CTB2016] Starburst>>
N:	3+1
Object:	MCld + Star forming region (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 3 and Band 7 observations of N=3 molecular clouds and N=1 starburst region in Zw II 40.
in source:	ZW II 40
Ref:	=2016ApJ...833L...6C
by	CONSIGLIO S.M. , TURNER J.L., BECK S., MEIER D.S.
	Astrophys. J., 833L, 6-6 (2016)
	ALMA reveals potential localized dust enrichment from massive star clusters in II Zw 40.
o	Fig. 2, Table 1: <[CTB2016] Cloud W> (Nos E, W, C), <[CTB2016] Starburst> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTB2017]
[CTB2017]	(Consiglio+Turner+Beck+, 2017)
Write:	<<[CTB2017] DN>>
N:	7
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	ALMA 12CO(3-2) and 13CO(3-2) observations of N=7 subclouds within the cloud [MTB2002] D in the dwarf spheroidal galaxy NGC 5253.
in source:	NGC 5253:[MTB2002] D = [MTB2002] D
Ref:	=2017ApJ...850...54C
by	CONSIGLIO S.M. , TURNER J.L., BECK S., MEIER D.S., SILICH S., ZHAO J.-H.
	Astrophys. J., 850, 54-54 (2017)
	ALMA CO(3-2) observations of star-forming filaments in a gas-poor dwarf spheroidal galaxy.
o	Fig. 5, Table 1: <[CTB2017] DN> (Nos D1-D7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTB81]
[CTB81]	(Chincarini+Tarenghi+Bettis, 1981)= (CH)
Write:	<<[CTB81] NNNA>>
N:	35 among 102
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	CA 0340-538 = ACO 3158
Ref:	=1981A&A....96..106C
by	CHINCARINI G. , TARENGHI M., BETTIS C.
	Astron. Astrophys., 96, 106-110 (1981)
	Observations of galaxies in the southern cluster CA 0340-538.
o	Table 1, text: <[CTB81] NNNA> N=35 among N>103
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTB95]
[CTB95]	(Clementini+Tosi+Bragaglia+, 1995)
Write:	<<[CTB95] AA CCC AN>>
N:	9
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Primary comparison stars in the field of 7 RR Lyrae.
Ref:	=1995MNRAS.275..929C
by	CLEMENTINI G. , TOSI M., BRAGAGLIA A., MERIGHI R., MACERONI C.
	Mon. Not. R. Astron. Soc., 275, 929-943 (1995)
	New pulsational properties of eight 'anomalous' RR Lyrae variables.
o	Table 2: <[CTB95] AA CCC AN> N=7.
Ref:	=2002MNRAS.336..841D
by	DI FABRIZIO L. , CLEMENTINI G., MARCONI M., CARRETTA E., IVANS I.I., BRAGAGLIA A., DI TOMASO S., MERIGHI R., SMITH H.A., SNEDEN C., TOSI M.
	Mon. Not. R. Astron. Soc., 336, 841-850 (2002)
	Anomalous RR Lyrae stars(?): CM Leonis.
o	Table 2, Fig.1: <[CTB95] CM Leo AN> (Nos C2-C3) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTC2002]
[CTC2002]	(Curiel+Trinidad+Canto+, 2002)
Write:	<<[CTC2002] VLA-mm>> <<[CTC2002] VLA-RN>>
N:	1+2
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	See also [TPG2001].
in source:	NAME Cep A
Ref:	=2002ApJ...564L..35C
by	CURIEL S. , TRINIDAD M.A., CANTO J., RODRIGUEZ L.F., TORRELLES J.M., HO P.T.P., PATEL N.A., GREENHILL L., GOMEZ J.F., GARAY G., HERNANDEZ L., CONTRERAS M.E., ANGLADA G.
	Astrophys. J., 564, 35-38 (2002)
	Detection of a candidate for the exciting source of the expanding water maser bubble in Cepheus A.
o	Table 2: <[CTC2002] VLA-mm> N=1, <[CTC2002] VLA-RN> (Nos R4, R5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTC2004]
[CTC2004]	(Comeron+Torra+Chiappini+, 2004)
Write:	<<[CTC2004] NNN>>
N:	195 among 202
Object:	* (SIMBAD class: Star)
Note:	NIR observations at the Calar Alto 1.23m telescope. Search for supergiant stars in the Milky Way.
Ref:	=2004A&A...425..489C
by	COMERON F. , TORRA J., CHIAPPINI C., FIGUERAS F., IVANOV V.D., RIBAS S.J.
	Astron. Astrophys., 425, 489-508 (2004)
	A search for late-type supergiants in the inner regions of the Milky Way.
o	Table 1: <[CTC2004] NNN> N=195 among (Nos 1-202).
=E=	Catalogue in electronic form as J/A+A/425/489
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTC2009]
[CTC2009]	(Chiagerbe+Tremblay+Capetti+, 2009)
Write:	<<[CTC2009] NNN>>
N:	37
Object:	Radio Galaxy Candidate (SIMBAD class: RadioG = Radio Galaxy)
Note:	Search for FRI radio galaxies between 1<z<2 based on the VLA FIRST catalogue in the COSMOS field.
Ref:	=2009ApJ...696.1103C
by	CHIABERGE M. , TREMBLAY G., CAPETTI A., MACCHETTO F.D., TOZZI P., SPARKS W.B.
	Astrophys. J., 696, 1103-1115 (2009)
	Low-power radio galaxies in the distant universe: a search for FR I at 1 < z < 2 in the COSMOS field.
o	Table 1: <[CTC2009] NNN> N=37 among (Nos 1-285).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTC2016]
[CTC2016]	(Castangia+Tarchi+Caccianiga+, 2016)
Write:	<<[CTC2016] {M\|C}N>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLBA 22GHz observations of N=5 H2O maser towards IRAS 15480-0344.
in source:	IRAS 15480-0344
Ref:	=2016A&A...586A..89C
by	CASTANGIA P. , TARCHI A., CACCIANIGA A., SEVERGNINI P., DELLA CECA R.
	Astron. Astrophys., 586A, 89-89 (2016)
	Water masers in Compton-thick AGN. I. Detailed study of the new water megamaser in IRAS 15480-0344.
o	Table 3: <[CTC2016] MN> (Nos M1-M2). Table 4: <[CTC2016] CN> (Nos C1-C2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTC2021]
[CTC2021]	(Cheng+Tan+Caselli+, 2021)
Write:	<<[CTC2021] Vela C CR1>> <<[CTC2021] Vela C CR1cNN>>
N:	1+11
Object:	Clump + Core (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA Bands 6 and 7 observations of N=1 dense clump in the Center Ridge of Vela C and N=11 cores in this clump. Use of Spitzer, WISE, Herschel archival data.
in source:	NAME Vela C Cloud
Ref:	=2021ApJ...916...78C
by	CHENG Y. , TAN J.C., CASELLI P., FISSEL L., ARCE H.G., FONTANI F., GOODSON M.D., LIU M., GALITZKI N.
	Astrophys. J., 916, 78-78 (2021)
	Star formation in a strongly magnetized cloud.
o	Fig. 2: <[CTC2021] Vela C CR1> N=1. Fig. 3, Table 1: <[CTC2021] Vela C CR1cNN> (Nos CR1c1-CR1c11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CTCS
CTCS	(Cerro Tololo obs., Curtis Schmidt telescope)
*****	Avoid the usage of CTCS, prefer BPS
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: CTCV
CTCV	(Calan Tololo, Cataclysmic Variable)
Write:	<<CTCV JHHMM+DDMM>>
Object:	Poss. Catacl. V* (SIMBAD class: CataclyV* = Cataclysmic Binary)
Note:	In ref. 1999A&A...350..379R CTCV objects are QSOs.
Ref:	=1999A&A...350..379R
by	ROSSA J. , TAPPERT C., AUGUSTEIJN T., MAZA J.
	Astron. Astrophys., 350, 379-380 (1999)
	Two new quasars at z = 1.90 and z = 0.15 from the Calan-Tololo Survey.
o	Table 1: <CTCV JHHMM+DDMM> N=3.
Ref:	=2004MNRAS.354..321T
by	TAPPERT C. , AUGUSTEIJN T., MAZA J.
	Mon. Not. R. Astron. Soc., 354, 321-331 (2004)
	Cataclysmic variables from the Calan-Tololo Survey - I. Photometric periods.
o	Table 1: <CTCV JHHMM+DDMM> N=6 added.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CTD
CTD	(Caltech obs., list D)
Write:	<<CTD NNN>>
N:	143
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ν = 1421MHz. HPBW = 33'
Ref:	=1965POVRO..12....1K
by	KELLERMANN K.I. , READ R.B.
	Publ. Owens Valley Obs., 12, 1-5 (1965)
	A continuum survey for discrete radio sources at 1421 MC/S.
o	Table 1: <CTD NNN> (Nos 1-143)
Details on Acronym: [CTD2007]
[CTD2007]	(Chary+Teplitz+Dickinson+, 2007)
Write:	<<[CTD2007] JHHMMSS.ss+DDMMSS.ss>>
N:	3
Object:	(IR) G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IR Spectrograph observations of the HUDF.
in source:	NAME HUDF
Ref:	=2007ApJ...665..257C
by	CHARY R.-R. , TEPLITZ H.I., DICKINSON M.E., KOO D.C., LE FLOC'H E., MARCILLAC D., PAPOVICH C., STERN D.
	Astrophys. J., 665, 257-264 (2007)
	Hubble Ultra Deep Field-JD2: mid-infrared evidence for a z ~ 2 luminous infrared galaxy.
o	Text: <[CTD2007] JHHMMSS.ss++DDMMSS.ss> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTD2010]
[CTD2010]	(Courbin+Tewes+Djorgovski+, 2010)
Write:	<<[CTD2010] SDSS J0013+1523 A>> <<[CTD2010] SDSS J0013+1523 GN>>
N:	2+2
Object:	Grav. lensed image of a G + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Keck NIRC2 photometry and LRIS spectroscopy of strong gravitational lensing by the QSO SDSS J001340.21+152312.0.
Ref:	=2010A&A...516L..12C
by	COURBIN F. , TEWES M., DJORGOVSKI S.G., SLUSE D., MAHABAL A., RERAT F., MEYLAN G.
	Astron. Astrophys., 516L, 12-12 (2010)
	First case of strong gravitational lensing by a QSO: SDSS J0013+1523 at z = 0.120.
o	Figs 2-3, Table 1: <[CTD2010] SDSS J0013+1523 A> (Nos A-B), <[CTD2010] SDSS J0013+1523 GN> (Nos G1-G2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTF2006]
[CTF2006]	(Colbert+Teplitz+Francis+, 2006)
Write:	<<[CTF2006] JHHMMSS.ss+DDMMSS.s>>
N:	3
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Spitzer Space Telescope observations of Ly-alpha sources associated with ClG J2143-4423. Three new possible Ly-alpha blob companions are found. See also [FWW96].
Ref:	=2006ApJ...637L..89C
by	COLBERT J.W. , TEPLITZ H., FRANCIS P., PALUNAS P., WILLIGER G.M., WOODGATE B.
	Astrophys. J., 637, 89-92 (2006)
	Ultraviolet-bright, high-redshift ultraluminous infrared galaxies.
o	T. 1, Fig.1 : Blob B6 is [FWW96] B6' = [PTF2004] J214242.63-443009.0 in SIMBAD.
o	Table 1: <[FWW96] BN> (Nos B8-B9) added. Table 1: <[CTF2006] JHHMMSS.ss+DDMMSS.s> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTF93]
[CTF93]	(Chen+Tokunaga+Fukui, 1993)= (IRAS)
Write:	<<[CTF93] NNN>>
N:	312
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	1st ref.: N=224, 2nd ref.: N=59, betw. Nos 1-312.
in source:	Orion Nebula:LDN 1641 = LDN 1641
Ref:	=1993ApJ...416..235C
by	CHEN H. , TOKUNAGA A.T., FUKUI Y.
	Astrophys. J., 416, 235-246 (1993)
	An IRAS sample from co-added images of L 1641.
o	[CTF93]50 = [MB91]21 ?
o	<[CTF93] NNN> N=224 among 312
Ref:	=1994ApJS...90..149C
by	CHEN H. , TOKUNAGA A.T.
	Astrophys. J., Suppl. Ser., 90, 149-172 (1994)
	Stellar density enhancements associated with IRAS sources in L1641.
o	Table 1: <[CTF93] NNN> N=59 among 312
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTG97]
[CTG97]	(Chen+Tafalla+Greene+, 1997)
Write:	<<[CTG97] A>> <<[CTG97] N>>
N:	3+8
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Objects in the embedded cluster around IRAS 20050+2720 Table 1: N=3 subclusters (Nos A-C) Table 2: N=8 sources (Nos 1-8) See also [CPE99].
Ref:	=1997ApJ...475..163C
by	CHEN H. , TAFALLA M., GREENE T.P., MYERS P.C., WILNER D.J.
	Astrophys. J., 475, 163-172 (1997)
	IRAS 20050+2720: an embedded young cluster associated with a multipolar outflow.
o	Table 1: <[CTG97] A> (Nos A-C). Table 2: <[CTG97] N> (Nos 1-8)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTH2000]
[CTH2000]	(Crosthwaite+Turner+Ho, 2000)
Write:	<<[CTH2000] JHHMMSS+DDMMSS>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=3 unresolved 21cm sources near IC 342, probably not associated with IC 342.
Ref:	=2000AJ....119.1720C
by	CROSTHWAITE L.P. , TURNER J.L., HO P.T.P.
	Astron. J., 119, 1720-1736 (2000)
	Structure in the neutral hydrogen disk of the spiral galaxy IC 342.
o	Galaxy A0355 = UGCA 86. p.1733: Holes in examples are not in SIMBAD.
o	Text: <[CTH2000] JHHMMSS+DDMMSS> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTH2008]
[CTH2008]	(Castangia+Tarchi+Henkel+, 2008)
Write:	<<[CTH2008] NGC 520 A>>
N:	7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	MERLIN and VLA observations of radio compact sources in NGC 520.
in source:	NGC 520
Ref:	=2008A&A...479..111C
by	CASTANGIA P. , TARCHI A., HENKEL C., MENTEN K.M.
	Astron. Astrophys., 479, 111-122 (2008)
	New H_{2}O masers in Seyfert and FIR bright galaxies II. The intermediate luminosity range.
o	Tables 4, 5: <[CTH2008] NGC 520 A> (Nos A-G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTH90]
[CTH90]	(Carral+Turner+Ho, 1990)
Write:	<<[CTH90] NGC NNNN CNN>> <<[CTH90] NGC NNNN CNNW>>
N:	28+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radiocomponents of 6 galaxies, format 'CNN' or 'CNNW'
in source:	NGC 520
in source:	NGC 660
in source:	NGC 2146
in source:	NGC 3628
in source:	NGC 4151
in source:	NGC 6240
Ref:	=1990ApJ...362..434C
by	CARRAL P. , TURNER J.L., HO P.T.P.
	Astrophys. J., 362, 434-442 (1990)
	15 GHz compact structure in galactic nuclei.
o	Table 2: NGC 3690 A, B = [GSW83] A, B
o	Table 2: <[CTH90] NGC 520 CN> (Nos C1-C5), <[CTH90] NGC 660 CN> (Nos C1-C2), <[CTH90] NGC 2146 CN> (Nos C1-C2), <[CTH90] NGC 3628 CNN> (Nos C1-C10), <[CTH90] NGC 4151 CN> (Nos C1-C6), <[CTH90] NGC 6240 CN> (Nos C1-C2).
Ref:	=1993MNRAS.263..471P
by	PEDLAR A. , KUKULA M.J., LONGLEY D.P.T., MUXLOW T.W.B., AXON D.J., BAUM S., O'DEA C., UNGER S.W.
	Mon. Not. R. Astron. Soc., 263, 471-480 (1993)
	The radio nucleus of NGC 4151 at 5 and 8 GHz.
o	Table 1: <[CTH90] NGC 4151 C7> added
Ref:	=1998ApJ...496..196U
by	ULVESTAD J.S. , ROY A.L., COLBERT E.J.M., WILSON A.S.
	Astrophys. J., 496, 196-202 (1998)
	A subparsec radio jet or disk in NGC 4151.
o	Pedlar et al., 1993 = [CTH90] in SIMBAD. p.199 : Component S1 in NGC 1068 = [GBO96] S1 in SIMBAD
o	text: <[CTH90] NGC 4151 C04W> (Nos C04E, C04W) added. Table 1: <[URC98] A> (Nos A-H). Table 2: <[URC98] AN> (Nos D1-D3, E1-E6, F1-F5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CTI
CTI	(CCD Transit Instrument)
Write:	<<CTI HHMMSS.s+DDMMSSA>>
N:	187
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	In format, coordinates are from equinox 1987.5, epoch 1990. 2 stars were already found in 1991ApJS...77..417K.
Ref:	=1994ApJS...94..749K
by	KIRKPATRICK J.D. , McGRAW J.T., HESS T.R., LIEBERT J., McCARTHY D.W.Jr
	Astrophys. J., Suppl. Ser., 94, 749-788 (1994)
	The luminosity function at the end of the main sequence: results of a deep, large-area, CCD survey for cool dwarfs.
o	CTI format: equinox 1987.5, epoch 1990.
o	Tables 1, 5: <CTI HHMMSS.s+DDMMSSA> N=187.
=E=	Catalogue in electronic form as J/ApJS/94/749
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CTIO
CTIO	(CTIO)
*****	Avoid the usage of CTIO, prefer [BSM2001]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CTIO
CTIO	(Cerro Tololo International Obs.)
Note:	CTIO 1230-275 = Tol 26 = Tol 1230-275 =
*****	Avoid the usage of CTIO, prefer Tol
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CTIO
CTIO	(Cerro Tololo Inter-american Obs.)
*****	Avoid the usage of CTIO, prefer UScoCTIO
Origin	of the Acronym: L (2001AJ....121.1040P)
Details on Acronym: CTIO85
CTIO85	(Cerro Tololo Inter-american Obs., 1985)
Write:	<<CTIO85 NNN>>
N:	280
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	UBV observations made by Massey and DeGioia-Eastwood in 1985 at the Cerro Tololo Inter-american Obs., published in 2001AJ....121..891P. N=280 stars in LH 2.
in source:	Magellanic Clouds:LMC:LH 2 = LH 2
Ref:	=2001AJ....121..891P
by	PARKER J.W. , ZARITSKY D., STECHER T.P., HARRIS J., MASSEY P.
	Astron. J., 121, 891-904 (2001)
	Ultraviolet and optical observations of OB associations and field stars in the southwest region of the Large Magellanic Cloud.
o	Table 1: <CTIO85 NNN> (Nos 1-280).
=E=	Catalogue in electronic form as J/AJ/121/891
Origin	of the Acronym: L (2001AJ....121..891P)
Details on Acronym: [CTL2020]
[CTL2020]	(Cheng+Tan+Liu+, 2020)
Write:	<<[CTL2020] G286cNN>>
N:	76
Object:	Dense Core (SIMBAD class: denseCore = Dense Core)
Note:	ALMA band 6 observations of N=76 continuum-defined dense cores in the massive protocluster GAL 286.21+00.17. Use of Herschel Hi-GAL data.
in source:	GAL 286.21+00.17
Ref:	=2020ApJ...894...87C
by	CHENG Y. , TAN J.C., LIU M., LIM W., ANDERSEN M.
	Astrophys. J., 894, 87-87 (2020)
	Gas kinematics of the massive protocluster G286.21+0.17 revealed by ALMA.
o	Table A1: <[CTL2020] G286cNN> (Nos G286c1-G286c76).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTL96]
[CTL96]	(Cristiani+Trentini+La Franca+, 1996)
Write:	<<[CTL96] HHMMSS.ss+DDMMSS.s>>
N:	180
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	The authors don't give any format to their list, so we use the the coordinates in the format: 'HHMMSS.ss+DDMMSS.s', with leading zero for HH and DD if necessary
Ref:	=1996A&A...306..395C
by	CRISTIANI S. , TRENTINI S., LA FRANCA F., ARETXAGA I., ANDREANI P., VIO R., GEMMO A.
	Astron. Astrophys., 306, 395-407 (1996)
	The optical variability of QSOs.
o	Table 1: <[CTL96] HHMMSS.ss+DDMMSS.s> N=180
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CTLGD
CTLGD	(Deep astrometric catalogue)
Write:	<<CTLGD NNNNN>>
N:	11598
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Cesco Observatory (Argentina) photographic imaging. Second (deeper) catalogue CtlgD of proper motions in the area of Blanco 1. See also CTLGM (main catalogue of positions and proper motions).
in source:	Cl Blanco 1
Ref:	=2011MNRAS.413.1024P
by	PLATAIS I. , GIRARD T.M., VIEIRA K., LOPEZ C.E., LOOMIS C., McLEAN B.J., POURBAIX D., MORAUX E., MERMILLIOD J.-C., JAMES D.J., CARGILE P.A., BARNES S.A., CASTILLO D.J.
	Mon. Not. R. Astron. Soc., 413, 1024-1035 (2011)
	A deep proper-motion survey of the nearby open cluster Blanco 1.
o	Table 1: <CTLGM NNNN> (Nos 1-6271). Table 3: <CTLGD NNNNN> (Nos 1-11598).
=E=	Catalogue in electronic form as <J/MNRAS/413/1024/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CTLGM
CTLGM	(Main Catalog)
Write:	<<CTLGM NNNN>>
N:	6271
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Cesco Observatory (Argentina) photographic imaging. Main catalogue CtlgM of positions and proper motions in the area of Blanco 1. See also CTLGD (second catalogue of proper motions).
in source:	Cl Blanco 1
Ref:	=2011MNRAS.413.1024P
by	PLATAIS I. , GIRARD T.M., VIEIRA K., LOPEZ C.E., LOOMIS C., McLEAN B.J., POURBAIX D., MORAUX E., MERMILLIOD J.-C., JAMES D.J., CARGILE P.A., BARNES S.A., CASTILLO D.J.
	Mon. Not. R. Astron. Soc., 413, 1024-1035 (2011)
	A deep proper-motion survey of the nearby open cluster Blanco 1.
o	Table 1: <CTLGM NNNN> (Nos 1-6271). Table 3: <CTLGD NNNNN> (Nos 1-11598).
=E=	Catalogue in electronic form as <J/MNRAS/413/1024/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CTM2001]
[CTM2001]	(Comeron+Torra+Mendez+, 2001)
Write:	<<[CTM2001] NN>>
N:	30
Object:	* (SIMBAD class: Star)
Note:	SUSI2 observations on ESO NTT. UBV photometry of NGC 253.
in source:	NGC 253
Ref:	=2001A&A...366..796C
by	COMERON F. , TORRA J., MENDEZ R.A., GOMEZ A.E.
	Astron. Astrophys., 366, 796-810 (2001)
	Possible star formation in the halo of NGC 253.
o	Table 2, Fig.2: <[CTM2001] NN> (Nos 1-30).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTM2006]
[CTM2006]	(Castander+Treister+Maza+, 2006)
Write:	<<[CTM2006] G>> <<[CTM2006] QSO A>>
N:	1+2
Object:	G + Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Magellan Clay telescope photometry/spectroscopy and VLT FORS2 spectroscopy of the CXOCY J220132.8-320144 lensing system which is composed of an edge-on spiral galaxy lensing a background QSO with 2 images A and B.
Ref:	=2006ApJ...652..955C
by	CASTANDER F.J. , TREISTER E., MAZA J., GAWISER E.
	Astrophys. J., 652, 955-962 (2006)
	CXOCY J220132.8-320144: an edge-on spiral gravitational lens.
o	Fig.2, Tables 1, 2: <[CTM2006] G>, <[CTM2006] QSO A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTM2010]
[CTM2010]	(Chiboucas+Tully+Marzke+, 2010)
Write:	<<[CTM2010] NNNNNNN>>
N:	101
Object:	G (SIMBAD class: Galaxy)
Note:	Keck LRIS spectroscopy of dwarf galaxy candidates in the core region of the Coma Cluster.
in source:	Coma Cluster = ACO 1656
Ref:	=2010ApJ...723..251C
by	CHIBOUCAS K. , TULLY R.B., MARZKE R.O., TRENTHAM N., FERGUSON H.C., HAMMER D., CARTER D., KHOSROSHAHI H.
	Astrophys. J., 723, 251-266 (2010)
	Keck/LRIS spectroscopic confirmation of Coma cluster dwarf galaxy membership assignments.
o	Table 2: <[CTM2010] NNNNNNN> N=101 among (Nos 10162-4042826).
Ref:	=2011ApJ...737...86C
by	CHIBOUCAS K. , TULLY R.B., MARZKE R.O., PHILLIPPS S., PRICE J., PENG E.W., TRENTHAM N., CARTER D., HAMMER D.
	Astrophys. J., 737, 86 (2011)
	Ultra-compact dwarfs in the Coma cluster.
o	Tables 2-4: <[CTM2010] NNNNNNN> N=78 among (Nos 10355-8039100).
=E=	Catalogue in electronic form as J/ApJ/723/251
=E=	Catalogue in electronic form as <J/ApJ/737/86/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CTOI
CTOI	(Community TESS Object of Interest)= (TIC)
Write:	<<CTOI NNNNNNNNNNN.NN>>
Object:	Poss. Planet (SIMBAD class: Planet_Candidate = Extra-solar Planet Candidate)
Note:	Community TESS Objects of Interest (CTOIs) are intended to be a mechanism for the community members to identify planetary systems or other potentially interesting objects discovered by TESS but not identified as a TESS Object of Interest (TOI) by the TESS project. The list of CTOIs is available at: https://exofop.ipac.caltech.edu/tess/view_ctoi.php
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CTP2007]
[CTP2007]	(Curran+Tzanavaris+Phihlstrom+, 2007) (Not yet in Simbad)
Write:	<<[CTP2007] QSO J0813+4813 abs N.NNNNN>>
N:	1
Object:	DLA
Ref:	=2007MNRAS.382.1331C
by	CURRAN S.J. , TZANAVARIS P., PIHLSTROM Y.M., WEBB J.K.
	Mon. Not. R. Astron. Soc., 382, 1331-1341 (2007)
	Relationships between the HI 21-cm line strength, MgII equivalent width and metallicity in damped Lyman α absorption systems.
o	Table 1: <[CTP2007] QSO J0813+4813 abs N.NNNNN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CTQ
CTQ	(Calan Tololo, QSO)
Write:	<<CTQ NNNNA>>
Object:	QSO (SIMBAD class: QSO = Quasar)
Note:	QSO in Calan-Tololo Survey, see CTS. (Nos 201-700) are also CTS NNN objects, but numbering of CTS QSOs is not following the numbering rule used by Maza&Co (see CTS), and needs the creation of a new acronym CTQ.
Ref:	=1993RMxAA..25...51M
by	MAZA J. , RUIZ M.T., GONZALEZ L.E., WISCHNJEWSKY M., ANTEZANA R.
	Rev. Mex. Astron. Astrofis., 25, 51-57 (1993)
	Calan-Tololo survey. V. Two hundred new southern quasars.
o	Table 1: <CTS NNN> (Nos 201-400) = <CTS ANN.NN> N=200 = <CTQ NNN> (Nos 201-400).
Ref:	=1995RMxAA..31..119M
by	MAZA J. , WISCHNJEWSKY M., ANTEZANA R., GONZALEZ L.E.
	Rev. Mex. Astron. Astrofis., 31, 119-129 (1995)
	Calan-Tololo survey. VI. One hundred new southern quasars.
o	Table 1: <CTS NNN> (Nos 401-500) = <CTS ANN.NN> = <CTQ NNN> (Nos 401-500).
Ref:	=1995RMxAA..31..159M
by	MAZA J. , ORTIZ P.F., WISCHNJEWSKY M., ANTEZANA R., GONZALEZ L.E.
	Rev. Mex. Astron. Astrofis., 31, 159-169 (1995)
	Calan-Tololo survey. VII. One hundred southern quasars.
o	Table 1: <CTS NNN> (Nos 501-600) = <CTS ANN.NN> = <CTQ NNN> (Nos 501-600).
Ref:	=1996RMxAA..32...35M
by	MAZA J. , WISCHNJEWSKY M., ANTEZANA R.
	Rev. Mex. Astron. Astrofis., 32, 35-45 (1996)
	CALAN-TOLOLO survey. VIII. One hundred southern quasars.
o	Table 1: <CTS NNN> (Nos 601-700) = <CTS ANN.NN> = <CTQ NNN> (Nos 601-700).
Ref:	=2000AJ....119.1083M
by	MORGAN N.D. , BURLEY G., COSTA E., MAZA J., PERSSON S.E., RUIZ M.T., SCHECHTER P.L., THOMPSON I., WINN J.N.
	Astron. J., 119, 1083-1089 (2000)
	CTQ 839: candidate for the smallest projected separation binary quasar.
o	Fig.1, Table 3: <[MBC2000] N> (Nos 1-8). Fig.1, Table 4: <CTQ NNNA> (Nos 839, 839A, 839B).
Ref:	=2001A&A...366..387L
by	LOPEZ S. , MAZA J., MASEGOSA J., MARQUEZ I.
	Astron. Astrophys., 366, 387-394 (2001)
	Slit spectroscopy of nine new (z>3) southern QSOs: damped Lyα and Lyman-limit systems.
o	Table 1: <CTQ NNNN> (Nos 1005, 1061) added. Table 2: <[LMM2001] QSO J0041-4936 abs N.NNNN> N=16 = <[LMM2001] CTQ 408 NN> (Nos 1-20). Table 3: <[LMM2001] QSO J0407-4410 abs N.NNNN> N=22 = <[LMM2001] CTQ 247 NN> (Nos 1-27). Table 4: <[LMM2001] QSO J1048-1637 abs N.NNNN> N=2 = <[LMM2001] CTQ 1061 N> (Nos 1-2). Table 5: <[LMM2001] QSO J0137-2707 abs N.NNNN> N=5 = <[LMM2001] CTQ 1005 N> (Nos 1-5). Table 6: <[LMM2001] QSO J1039-2313 abs N.NNNN> N=10 = <[LMM2001] CTQ 460 NN> (Nos 1-10). Table 7: <[LMM2001] QSO J1235-3050 abs N.NNNN> N=7 = <[LMM2001] CTQ 314 N> (Nos 1-7). Table 8: <[LMM2001] QSO J1456-1938 abs N.NNNN> N=4 = <[LMM2001] CTQ 476 N> (Nos 1-5). Table 9: <[LMM2001] QSO J1342-1355 abs N.NNNN> N=3 = <[LMM2001] CTQ 325 N> (Nos 1-4). Table 10: <[LMM2001] QSO J1113-1533 abs N.NNNN> N=3 = <[LMM2001] CTQ 298 N> (Nos 1-3).
Details on Acronym: [CTR2020]
[CTR2020]	(Collins+Tollerud+Rich+, 2020)
Write:	<<[CTR2020] JDD.dddddd+DD.dddddd>>
N:	627
Object:	RGB* (SIMBAD class: Star)
Note:	Subaru Suprime-Cam photometry and Keck II DEIMOS spectroscopy of N=627 stars in the M 31 satellite galaxy Andromeda XIX.
in source:	And XIX
Ref:	=2020MNRAS.491.3496C
by	COLLINS M.L.M. , TOLLERUD E.J., RICH R.M., IBATA R.A., MARTIN N.F., CHAPMAN S.C., GILBERT K.M., PRESTON J.
	Mon. Not. R. Astron. Soc., 491, 3496-3514 (2020)
	A detailed study of Andromeda XIX, an extreme local analogue of ultradiffuse galaxies.
o	Table A1: <[CTR2020] JDD.dddddd+DD.dddddd> N=83.
=E=	Catalogue in electronic form as <J/MNRAS/491/3496/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTR95]
[CTR95]	(Combi+Testori+Romero+, 1995)
Write:	<<[CTR95] NN>>
N:	14
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
in source:	Ass Sco OB 2
Ref:	=1995A&A...296..514C
by	COMBI J.A. , TESTORI J.C., ROMERO G.E., COLOMB F.R.
	Astron. Astrophys., 296, 514-522 (1995)
	1435MHz continuum observations of Upper-Scorpius.
o	Table 1: <[CTR95] NN> (Nos 1-14)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CTS
CTS	(Calan Tololo Survey)= (CT) = CTQ
Write:	<<CTS NNN>> <<CTS 1NNNa>> <<CTS ANN.NN>> <<CTS ANN.NNa>>
N:	120+500+42
Object:	Seyfert G + HII G + QSO (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Format 'NNNN': (Nos 1-120): Seyfert galaxies (Format could be between No. 1 and No. 199 for Seyfert G). (Nos 201-700): QSOs (Format could be between No. 200 and No. 999 for QSOs). See also CTQ. (Nos 1001-1042): HII galaxies (Format is always a 4 digits format, first digit '1' for HII G), Nos 1024 and 1026 have 2 components 'a' and 'b'. Format 'ANN.NN' is explained in ref. 1989ApJS...69..349M, fig. 1: Ex.: B25.02 is the second object found on the 25th plate of strip B. Finding charts
Ref:	=1989ApJS...69..349M
by	MAZA J. , RUIZ M.T., GONZALEZ L.E., WISCHNJEWSKY M.
	Astrophys. J., Suppl. Ser., 69, 349-352 (1989)
	Calan-Tololo survey. I. Seyfert 1 galaxies.
o	<CTS NN> (Nos 1-30) = <CTS ANN.NN>
Ref:	=1991A&AS...89..389M
by	MAZA J. , RUIZ M.T., PENA M., GONZALEZ L.E., WISCHNJEWSKY M.
	Astron. Astrophys., Suppl. Ser., 89, 389-397 (1991)
	Calan-Tololo survey. III. HII galaxies.
o	<CTS 10NNa> (Nos 1001-1023, 1024a-b, 1025-1035, 1036a-b, 1037-1042) = <CTS ANN.NN>
Ref:	=1992RMxAA..24..147M
by	MAZA J. , RUIZ M.T., GONZALEZ L.E., WISCHNJEWSKY M.
	Rev. Mex. Astron. Astrofis., 24, 147-None (1992)
	Calan-Tololo survey II : Seyfert 1 galaxies.
o	<CTS NN> (Nos 31-70) = <CTS ANN.NN>
Ref:	=1993RMxAA..25...51M
by	MAZA J. , RUIZ M.T., GONZALEZ L.E., WISCHNJEWSKY M., ANTEZANA R.
	Rev. Mex. Astron. Astrofis., 25, 51-57 (1993)
	Calan-Tololo survey. V. Two hundred new southern quasars.
o	Table 1: <CTS NNN> (Nos 201-400) = <CTS ANN.NN> N=200 = <CTQ NNN> (Nos 201-400).
Ref:	=1994RMxAA..28..187M
by	MAZA J. , RUIZ M.T., GONZALEZ L.E., WISCHNJEWSKY M., ANTEZANA R.
	Rev. Mex. Astron. Astrofis., 28, 187-195 (1994)
	Calan-Tololo survey. IV. Seyfert 1 galaxies.
o	(Erratum) 1995 vol. 31, p. 87
o	Table I : coordinates are for 2000.0, not 1950.0
o	<CTS NNN> (Nos 71-120) = <CTS ANN.NN>
Ref:	=1995RMxAA..31..119M
by	MAZA J. , WISCHNJEWSKY M., ANTEZANA R., GONZALEZ L.E.
	Rev. Mex. Astron. Astrofis., 31, 119-129 (1995)
	Calan-Tololo survey. VI. One hundred new southern quasars.
o	Table 1: <CTS NNN> (Nos 401-500) = <CTS ANN.NN> = <CTQ NNN> (Nos 401-500).
Ref:	=1995RMxAA..31..159M
by	MAZA J. , ORTIZ P.F., WISCHNJEWSKY M., ANTEZANA R., GONZALEZ L.E.
	Rev. Mex. Astron. Astrofis., 31, 159-169 (1995)
	Calan-Tololo survey. VII. One hundred southern quasars.
o	Table 1: <CTS NNN> (Nos 501-600) = <CTS ANN.NN> = <CTQ NNN> (Nos 501-600).
Ref:	=1996RMxAA..32...35M
by	MAZA J. , WISCHNJEWSKY M., ANTEZANA R.
	Rev. Mex. Astron. Astrofis., 32, 35-45 (1996)
	CALAN-TOLOLO survey. VIII. One hundred southern quasars.
o	Table 1: <CTS NNN> (Nos 601-700) = <CTS ANN.NN> = <CTQ NNN> (Nos 601-700).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CTS
CTS	(Capellaro+Turatto+Sabbadin)
Write:	<<PN CTS N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	CTS 1 = PN G019.8+05.6
Ref:	=1989IAUS..131...61C
by	CAPPELLARO E. , TURATTO M., SABBADIN F.
	131st Symposium of the IAU held in Mexico City, Mexico, October 5-9, 1987. Ed S. Torres-Peimbert. Planetary Nebulae, 131, 61-None (1989)
	A new planetary nebula.
o	= PN G019.8+05.6
o	<PN CTS N> (No. 1).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CTS2002]
[CTS2002]	(Contini+Treyer+Sullivan+, 2002)
Write:	<<[CTS2002] NN>>
N:	68
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Sample of UV-selected intermediate redshift galaxies.
Ref:	=2002MNRAS.330...75C
by	CONTINI T. , TREYER M.A., SULLIVAN M., ELLIS R.S.
	Mon. Not. R. Astron. Soc., 330, 75-91 (2002)
	Chemical abundances in a UV-selected sample of galaxies.
o	Table 1: <[CTS2002] NN> (Nos 1-68).
=E=	Catalogue in electronic form as J/MNRAS/330/75
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTS2017]
[CTS2017]	(Collins+Tollerud+Sand+, 2017)
Write:	<<[CTS2017] NN>>
N:	28
Object:	* (SIMBAD class: Star)
Note:	Keck II DEIMOS spectro-photometric observations of N=28 stars in the field of Leo V dwarf galaxy. See also [WBE2009].
in source:	NAME Leo V
Ref:	=2017MNRAS.467..573C
by	COLLINS M.L.M. , TOLLERUD E.J., SAND D.J., BONACA A., WILLMAN B., STRADER J.
	Mon. Not. R. Astron. Soc., 467, 573-585 (2017)
	Dynamical evidence for a strong tidal interaction between the Milky Way and its satellite, Leo V.
o	Table 1: <[CTS2017] NN> N=28 among (Nos 10-62).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTS93]
[CTS93]	(Chen+Tokunanga+Strom+, 1993)
Write:	<<[CTS93] NNN>> <<[CTS93] SNN>> <<[CTS93] CNN>>
N:	34+15+40
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Table 3: (Nos N1-N34), IR in LDN 1641N. Table 4: (Nos S1-S15), IR in KMS 11 (named Strom 11 by the authors). Table 5: (Nos C1-C40), IR in LDN 1641C.
in source:	Orion Nebula:LDN 1641 = LDN 1641
Ref:	=1993ApJ...407..639C
by	CHEN H. , TOKUNAGA A.T., STROM K.M., HODAPP K.-W.
	Astrophys. J., 407, 639-648 (1993)
	Infrared and optical imaging of IRAS sources with CO outflow: a snapshot of early star formation.
o	Table 3: <[CTS93] ANN> (Nos N1-N34). Table 4: <[CTS93] ANN> (Nos S 1-S15). Table 5: <[CTS93] ANN> (Nos C1-C40)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CTSS
CTSS	(Capellaro+Turatto+Salvadori+Sabbadin)
Write:	<<PN CTSS N>>
N:	4
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	CTSS 1 = PK 043+02 1, CTSS 2 = PN G 044.1+05.8 = PK 044+05 2, CTSS 3 = Sh 2-78 = PN G 046.8+03.8 = PK 046+03 1, CTSS 4 = PN G 046.8+02.9 = PK 046+02 1
Ref:	=1990A&AS...86..503C
by	CAPPELLARO E. , TURATTO M., SALVADORI L., SABBADIN F.
	Astron. Astrophys., Suppl. Ser., 86, 503-None (1990)
	Four newly identifield planetary nebulae in the Palomar plate 18h48m +12.
o	<PN CTSS N> (Nos 1-4).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CTT2001]
[CTT2001]	(Clowe+Trentham+Tonry, 2001) (Not yet in Simbad)
Write:	<<[CTT2001] BN>> <<[CTT2001] N>>
N:	9+3
Object:	Red G (SIMBAD class: Galaxy)
Note:	Fig.4: N=9 red galaxies (Nos B1-B9), and N=3 candidate red galaxies (Nos 1-3) in the field of the lens system MITG J2019+1127.
Ref:	=2001A&A...369...16C
by	CLOWE D. , TRENTHAM N., TONRY J.
	Astron. Astrophys., 369, 16-25 (2001)
	Weak lensing observations of the ``dark'' cluster MG 2016+112.
o	MG 2016+112 = MITG J2019++1127
o	Fig.4: <[CTT2001] BN> (Nos B1-B9), <[CTT2001] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CTT2022]
[CTT2022]	(Cheng+Tan+Tobin+, 2022)
Write:	<<[CTT2022] G286dNN>>
N:	38
Object:	Protostellar disk (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	ALMA band 6 observations of N=38 protostellar disks in the central region of the massive protocluster G286.21+0.17. See also [CTL2020].
in source:	GAL 286.21+00.17
Ref:	=2022ApJ...940..124C
by	CHENG Y. , TAN J.C., TOBIN J.J., FEDRIANI R., ANDERSEN M., WANG J.
	Astrophys. J., 940, 124 (2022)
	The Disk Population in a Distant Massive Protocluster.
o	Fig. 2, Table 1: <[CTT2022] G286dNN> (Nos G286d1-G286d38).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [CTW2005]
[CTW2005]	(Cleary+Taylor+Waldram+, 2005)
Write:	<<[CTW2005] JHHMM+DDMM>>
N:	102
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Very Small Array (VSA) 33 GHz observations of 8 fields previously observed with the Ryle Telescope at 15 GHz
Ref:	=2005MNRAS.360..340C
by	CLEARY K.A. , TAYLOR A.C., WALDRAM E., BATTYE R.A., DICKINSON C., DAVIES R.D., DAVIS R.J., GENOVA-SANTOS R., GRAINGE K., JONES M.E., KNEISSL R., POOLEY G.G., REBOLO R., RUBINO-MARTIN J.A., SAUNDERS R.D.E., SCOTT P.F., SLOSAR A., TITTERINGTON D., WATSON R.A.
	Mon. Not. R. Astron. Soc., 360, 340-353 (2005)
	Source subtraction for the extended Very Small Array and 33-GHz source count estimates.
o	(Erratum) erratum vol. 386, p. 1759 (2008)
o	Table A1: <[CTW2005] JHHMM+DDMM> N=102.
=E=	Catalogue in electronic form as J/MNRAS/360/340
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CU95]
[CU95]	(Cunow+Ungruhe, 1995)
Write:	<<[CU95] ACO NNNN NN>>
N:	59+43
Object:	G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Photometry in the fields of 8 ACO clusters: the catalog contains 59 galaxies and 43 . Table 2: format 'ACO 2690 NN', (Nos 1-11), N = 7 G + 4 Table 3: format 'ACO 4074 N', (Nos 1-9), N = 7 G + 2 * Table 4: format 'ACO 2749 N', (Nos 1-9), N = 6 G + 3 * Table 5: format 'ACO 80 NN', (Nos 1-10), N = 8 G + 2 * Table 6: format 'ACO 2829 N', (Nos 1-7), N = 5 G + 2 * Table 7: format 'ACO 2871 N', (Nos 1-9), N = 6 G + 3 * Table 8: format 'ACO 3195 N', (Nos 1-6), N = 4 G + 2 * Table 9: format 'ACO 3703 NN', (Nos 1-41), N = 16 G + 25 *
in source:	ACO 2690
in source:	ACO 4074
in source:	ACO 2749
in source:	ACO 80
in source:	ACO 2829
in source:	ACO 2871
in source:	ACO 3195
in source:	ACO 3703
Ref:	=1995A&AS..112..213C
by	CUNOW B. , UNGRUHE R.
	Astron. Astrophys., Suppl. Ser., 112, 213-219 (1995)
	Photometric CCD sequences in 8 southern Abell clusters.
o	Tables 2 to 9: <[CU95] ACO NNNN NN> N=59+43
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Cud
Cud	(Cudworth+)
*****	Avoid the usage of Cud, prefer COS
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CUD2008]
[CUD2008]	(Cardamone+Urry+Damen+, 2008)
Write:	<<[CUD2008] NNNN>>
N:	1017
Object:	X AGN (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	MUSYC ECDF-S X-ray source catalogue from Chandra data.
in source:	NAME CDFS
Ref:	=2008ApJ...680..130C
by	CARDAMONE C.N. , URRY C.M., DAMEN M., VAN DOKKUM P., TREISTER E., LABBE I., VIRANI S.N., LIRA P., GAWISER E.
	Astrophys. J., 680, 130-142 (2008)
	Mid-infrared properties and color selection for X-Ray-detected active galactic nuclei in the MUSYC Extended Chandra Deep Field-South.
o	Table 1: <[CUD2008] NNNN> (Nos 1-1017).
=E=	Catalogue in electronic form as <J/ApJ/680/130/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CUDSS
CUDSS	(Canada-UK Deep Submm Survey)= (CFRS)
Write:	<<CUDSS HH.NN>>
N:	23+27
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	CUDSS SCUBA Submm survey. In the format HH stands for hours field. See also [ELG99].
Ref:	=2000AJ....120.2244E
by	EALES S. , LILLY S., WEBB T., DUNNE L., GEAR W., CLEMENTS D., YUN M.
	Astron. J., 120, 2244-2268 (2000)
	The Canada-UK deep submillimeter survey. IV. The survey of the 14 hour field.
o	Tables 2, 3: <CUDSS HH.NN> (Nos 14.1 to 14.21).
Ref:	=2003ApJ...587...41W
by	WEBB T.M. , EALES S.A., LILLY S.J., CLEMENTS D.L., DUNNE L., GEAR W.K., IVISON R.J., FLORES H., YUN M.
	Astrophys. J., 587, 41-54 (2003)
	The Canada-UK deep submillimeter survey. VI. The 3 hour field.
o	HDF 850.1 = [HSD98] HDF850.1
o	Tables 1, 2: <CUDSS HH.NN> (Nos 03.1 to 03.27).
Ref:	=2003MNRAS.341.1217W
by	WASKETT T.J. , EALES S.A., GEAR W.K., PUCHNAREWICZ E.M., LILLY S., FLORES H., WEBB T., CLEMENTS D., STEVENS J.A., THUAN T.X.
	Mon. Not. R. Astron. Soc., 341, 1217-1225 (2003)
	XMM-Newton surveys of the Canada-France Redshift Survey fields - I. The submillimetre/X-ray relation.
o	Fig. 2: <CUDSS HH.NN> (Nos 14.22, 14.23) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Cul
Cul	(Culgoora obs.)
Write:	<<Cul HHMM+DDA>> <<Cul HHMM+DDd>>
N:	2214
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	1982PASAu...4..278S: components A, B, C to some sources are introduced. 1995AuJPh..48..143S: final updated and recalibrated list of sources
Ref:	=1973AuJPA..27....1S
by	SLEE O.B. , HIGGINS C.S.
	Australian J. Phys. Astrophys. Suppl., 27, 1-43 (1973)
	Culgoora-1 list of radio source measurements at 80 MHz.
o	Table 5: <Cul HHMM+DD> N=777
Ref:	=1975AuJPA..36....1S
by	SLEE O.B. , HIGGINS C.S.
	Australian J. Phys. Astrophys. Suppl., 36, 1-60 (1975)
	Culgoora-2 list of radio source measurements at 80 MHz.
o	Tables 3, 4: <Cul HHMM+DDA>, <Cul HHMM+DDd>, N=1748.
Ref:	=1977AuJPA..43....1S
by	SLEE O.B.
	Australian J. Phys. Astrophys. Suppl., 43, 1-123 (1977)
	Culgoora-3 list of radio source measurements.
o	<Cul HHMM+DD> N=99
Ref:	=1982PASAu...4..278S
by	SLEE O.B. , SIEGMAN B.C., MULHALL P.S.
	Proc. Astron. Soc. Australia, 4, 278-307 (1982)
	Spectra, dimensions and luminosities of radio sources in the Culgoora-3 list.
o	Table 7: <Cul HHMM+DDA>
Ref:	=1995AuJPh..48..143S
by	SLEE O.B.
	Australian J. Phys., 48, 143-186 (1995)
	Radio sources observed with the Culgoora circular array.
o	<Cul HHMM+DDd> N=2214
=E=	Catalogue in electronic form as VIII/35
Details on Acronym: [CUS2014]
[CUS2014]	(Csengeri+Urquhart+Schuller+, 2014)= (ATLASGAL)
Write:	<<[CUS2014] GLLL.llll+BB.bbbb>>
N:	10861
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	N=10861 compact submillimiter sources from the full ATLASGAL survey, using the Gaussclumps algorithm. For more information, see: http://www3.mpifr-bonn.mpg.de/div/atlasgal/
Ref:	=2014A&A...565A..75C
by	CSENGERI T. , URQUHART J.S., SCHULLER F., MOTTE F., BONTEMPS S., WYROWSKI F., MENTEN K.M., BRONFMAN L., BEUTHER H., HENNING Th., TESTI L., ZAVAGNO A., WALMSLEY M.
	Astron. Astrophys., 565A, 75-75 (2014)
	The ATLASGAL survey: a catalog of dust condensations in the Galactic plane.
o	Table 1: <[CUS2014] GLLL.llll+BB.bbbb> N=10861.
=E=	Catalogue in electronic form as J/A+A/565/A75
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CUYS
CUYS	(CIDA-UCM-Yale Survey)
Write:	<<CUYS JHHMMSS+DDMMSS>>
N:	183
Object:	ELG (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	Observations at the 1-m Schmidt telescope at the Venezuelan Astronomical Observatory. CIDA (Centro de Investigationes De Astronomia), UCM (Universidad Complutense de Madrid) and Yale University Survey for Emission-Line Galaxies.
Ref:	=2005MNRAS.359..930B
by	BONGIOVANNI A. , BRUZUAL G., MAGRIS G., GALLEGO J., GARCIA-DABO C.E., COPPI P., SABBEY C.
	Mon. Not. R. Astron. Soc., 359, 930-940 (2005)
	The CIDA-UCM-Yale shallow survey for emission-line galaxies.
o	Table 1: <CUYS JHHMMSS+DDMMSS> N=427.
=E=	Catalogue in electronic form as J/MNRAS/359/930
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CUZ2012]
[CUZ2012]	(Coe+Umetsu+Zitrin+, 2012)
Write:	<<[CUZ2012] DDD.ddddd+DD.ddddd>> <<[CUZ2012] NNa>>
N:	308+30
Object:	G + Grav. lensed image of a G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST ACS and MMT Hectospec observations of ACO 2261.
in source:	ACO 2261
Ref:	=2012ApJ...757...22C
by	COE D. , UMETSU K., ZITRIN A., DONAHUE M., MEDEZINSKI E., POSTMAN M., CARRASCO M., ANGUITA T., GELLER M.J., RINES K.J., DIAFERIO A., KURTZ M.J., BRADLEY L., KOEKEMOER A., ZHENG W., NONINO M., MOLINO A., MAHDAVI A., LEMZE D., INFANTE L., OGAZ S., MELCHIOR P., HOST O., FORD H., GRILLO C., ROSATI P., JIMENEZ-TEJA Y., MOUSTAKAS J., BROADHURST T., ASCASO B., LAHAV O., BARTELMANN M., BENITEZ N., BOUWENS R., GRAUR O., GRAVES G., JHA S., JOUVEL S., KELSON D., MOUSTAKAS L., MAOZ D., MENEGHETTI M., MERTEN J., RIESS A., RODNEY S., SEITZ S.
	Astrophys. J., 757, 22 (2012)
	CLASH: precise new constraints on the mass profile of the galaxy cluster A2261.
o	Table 2: <[CUZ2012] DDD.ddddd+DD.ddddd> N=308 ; Table 3: <[CUZ2012] NNa> N=30 among (Nos 1a-1b to 12a-12b).
=E=	Catalogue in electronic form as <J/ApJ/757/22/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CV
CV	(Cataclysmic Variable)
*****	Avoid the usage of CV, prefer [CGC98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CV
CV	(Cordoba obs., Variable)
Write:	<<CV NNN>>
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	3 V* are found in 1992PAZh...18.1002K: Nos 374, 394, 414
Rem:	V* Nomenclature.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CV
CV	(Coma Void)
Write:	<<NAME CV N>>
N:	1
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Note:	N=1 Carbon star, named 'CV 5' by the authors
Ref:	=1997AJ....113.1022M
by	MOODY J.W. , GREGORY S.A., SOUKUP M.S., JADERLUND E.C.
	Astron. J., 113, 1022-1025 (1997)
	Discovery of a faint carbon star at high galactic latitude.
o	<NAME CV 5>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CV98]
[CV98]	(Chupina+Vereshchagin, 1998)
Write:	<<[CV98] NN>>
N:	5 among <60
Object:	Group of * (SIMBAD class: Association = Association of Stars)
Note:	Table 2: stellar groups in M 67 with more than 5 members, N=5 among (Nos 32-60)
in source:	NGC 2682 = M 67
Ref:	=1998A&A...334..552C
by	CHUPINA N.V. , VERESHCHAGIN S.V.
	Astron. Astrophys., 334, 552-557 (1998)
	Stellar clumps within the corona in the open cluster M 67.
o	Table 1: numbering from the catalogue V/52: 'Cl* NGC 2682 FA NNNN'
o	Table 2: <[CV98] NN> N=5 among (Nos 32-60)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CV99]
[CV99]	(Christian+Vennes, 1999) (Not yet in Simbad)
Write:	<<[CV99] N>>
N:	3
Object:	* (SIMBAD class: Star)
Note:	Finding chart of EUVE J1438-432. (Nos 1-3) are 3 stars in the field of EUVE. No. 1 = WT 486, No. 2 = WT 487.
Ref:	=1999AJ....117.1852C
by	CHRISTIAN D.J. , VENNES S.
	Astron. J., 117, 1852-1856 (1999)
	Detection of a strong stellar flare from EUVE J1438-432.
o	Fig.1: <[CV99] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CVB
CVB	(C. Van Breukelen+)
*****	Avoid the usage of CVB, prefer [VCB2006]
Origin	of the Acronym: L (2007MNRAS.382..971V)
Details on Acronym: [CVB2008]
[CVB2008]	(Croft+Van Breugel+Brown+, 2008)
Write:	<<[CVB2008] Source A>>
N:	5
Object:	rG (SIMBAD class: RadioG = Radio Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLA 1.4GHz and Keck NIRC/LRIS observations of radio galaxies in the Bootes field.
in source:	NAME Bootes Field
Ref:	=2008AJ....135.1793C
by	CROFT S. , VAN BREUGEL W., BROWN M.J.I., DE VRIES W., DEY A., EISENHARDT P., JANNUZI B., ROTTGERING H., STANFORD S.A., STERN D., WILLNER S.P.
	Astron. J., 135, 1793-1802 (2008)
	Radio-loud high-redshift protogalaxy candidates in Bootes.
o	Table 1: <[CVB2008] Source A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CVB2009]
[CVB2009]	(Campisi+Vignali+Brusa+, 2009)
Write:	<<[CVB2009] NNNN>> <<[CVB2009] XID NNN>>
N:	14+149
Object:	Poss. AGN + (X) (SIMBAD class: X = X-ray Source)
Note:	NTT 3.5m telescope NIR and Chandra observations of the "Daddi field" centered on 14 49 29 +09 00 00.
Ref:	=2009A&A...501..485C
by	CAMPISI M.A. , VIGNALI C., BRUSA M., DADDI E., COMASTRI A., POZZETTI L., ALEXANDER D.M., RENZINI A., ARIMOTO N., KONG X.
	Astron. Astrophys., 501, 485-494 (2009)
	On the nature of red galaxies: the Chandra perspective.
o	Table 1: <[CVB2009] NNNN> N=14 among (Nos 1557-4012). Table A.1: <[CVB2009] XID NNN> (Nos 1-149).
=E=	Catalogue in electronic form as <J/A+A/501/485/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CVC2006]
[CVC2006]	(Corbin+Vacca+Cid Fernandes+, 2006)
Write:	<<[CVC2006] JHHMMSS.ss+DDMMSS.ss>>
N:	10
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST ACS-HRC observations of SDSS galaxies. N=10 young massive star cluster candidates are found in 6 galaxies.
in source:	SDSS J013352.0+134209.0
in source:	SDSS J023628.0-005829.0
in source:	SDSS J111934.0+513012.0
in source:	SDSS J112742.0+641001.0
in source:	SDSS J113341.0+634925.0
in source:	SDSS J115247.0-004007.0
Ref:	=2006ApJ...651..861C
by	CORBIN M.R. , VACCA W.D., CID FERNANDES R., HIBBARD J.E., SOMERVILLE R.S., WINDHORST R.A.
	Astrophys. J., 651, 861-873 (2006)
	Ultracompact blue dwarf galaxies: Hubble Space Telescope imaging and stellar population analysis.
o	The 2 components A and B of HS 0822+3542 = [PKP2003] HS 0822+3542 a and b in SIMBAD.
o	Table 5: <[CVC2006] JHHMMSS.ss+DDMMSS.ss> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CVC2010]
[CVC2010]	(Carraro+Vazquez+Costa+, 2010) (Not yet in Simbad)
Write:	<<[CVC2010] VdB-Hagen 04 NNNN>> <<[CVC2010] Ruprecht 30 NNNN>>
N:	71+193
Object:	* (SIMBAD class: Star)
Note:	CTIO 1.0m telescope observations of Cl VDBH 4 and Ruprecht 30.
in source:	Cl VDBH 4
in source:	Cl Ruprecht 30
Ref:	=2010ApJ...718..683C
by	CARRARO G. , VAZQUEZ R.A., COSTA E., PERREN G., MOITINHO A.
	Astrophys. J., 718, 683-694 (2010)
	The edge of the young Galactic disk.
o	Table 3: <[CVC2010] VdB-Hagen 04 NNNN> N=71 among (Nos 29-3885). Table 4: <[CVC2010] Ruprecht 30 NNNN> N=193 among (Nos 57-6107).
=E=	Catalogue in electronic form as <J/ApJ/718/683/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CVD2018]
[CVD2018]	(Cohen+Van Dokkum+Danieli+, 2018)
Write:	<<[CVD2018] NGCNNNN-DFNN>> <<[CVD2018] M96-DFNN>>
N:	23
Object:	LSB (SIMBAD class: LowSurfBrghtG = Low Surface Brightness Galaxy)
Note:	HST ACS observations of N=23 very low surface brightness LSB) galaxies in the fields of N=4 neaby galaxy groups. Use of the Dragonfly Nearby Galaxy Survey.
in source:	NGC 1052
in source:	NGC 1084
in source:	NGC 4258
in source:	M 96
Ref:	=2018ApJ...868...96C
by	COHEN Y. , VAN DOKKUM P., DANIELI S., ROMANOWSKY A.J., ABRAHAM R., MERRITT A., ZHANG J., MOWLA L., KRUIJSSEN J.M.D., CONROY C., WASSERMAN A.
	Astrophys. J., 868, 96-96 (2018)
	The Dragonfly Nearby Galaxies Survey. V. HST/ACS observations of 23 low surface brightness objects in the fields of NGC 1052, NGC 1084, M96, and NGC 4258.
o	Tables 1-3, Figs. 1-4: <[CVD2018] NGC1052-DFN> N=6 among (Nos 1-8), <[CVD2018] NGC1084-DF1> N=1, <[CVD2018] NGC4258-DFN> N=5 among (Nos 1-6), <[CVD2018] M96-DFNN> (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CVH2005]
[CVH2005]	(Corbin+Vacca+Hibbard+, 2005) (Not yet in Simbad)
Write:	<<[CVH2005] HS 0822+3542 A>> <<[CVH2005] N>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	HST observations of HS 0822+3542: N=2 components and 6 point-sources. See also [PKP2003].
in source:	HS 0822+3542
Ref:	=2005ApJ...629L..89C
by	CORBIN M.R. , VACCA W.D., HIBBARD J.E., SOMERVILLE R.S., WINDHORST R.A.
	Astrophys. J., 629, 89-92 (2005)
	Hubble space telescope imaging of the ultracompact blue dwarf galaxy HS 0822+3542: an assembling galaxy in a local void.
o	The 2 components A and B of HS 0822+3542 = [PKP2003] HS 0822+3542 a and b in SIMBAD.
o	Fig.1, Table 1: <[CVH2005] HS 0822+3542 A> (Nos A-B), <[CVH2005] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CVH2006]
[CVH2006]	(Chiosi+Vallenari+Held+, 2006)
Write:	<<[CVH2006] NNNA>>
N:	164+311+2
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	ESO 2.2m telescope WFI observations and use of archival OGLEII data. N=164 associations and 311 clusters in the central part of the SMC are studied. N=2 super-shells 37A and 304A are also detected.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2006A&A...452..179C
by	CHIOSI E. , VALLENARI A., HELD E.V., RIZZI L., MORETTI A.
	Astron. Astrophys., 452, 179-193 (2006)
	Age distribution of young clusters and field stars in the Small Magellanic Cloud.
o	Table 2: <[CVH2006] NNN> N=164+311 among (Nos 60-888).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CVI2002]
[CVI2002]	(Cornelisse+Verbunt+In't Zand+, 2002)
Write:	<<[CVI2002] SAX JHHMM.m+DDMM A>>
N:	5+3+9+8
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS observations. Search for candidate persistent sources for four X-ray bursters.
Ref:	=2002A&A...392..931C
by	CORNELISSE R. , VERBUNT F., IN'T ZAND J.J.M., KUULKERS E., HEISE J.
	Astron. Astrophys., 392, 931-936 (2002)
	Chandra follow-up of bursters with low persistent emission.
o	In table 2, SAX 1752.3-3128 is a misprint for SAX J1752.3-3138.
o	Table 3: <[CVI2002] SAX JHHMM.m+DDMM A> N=5+3+9+8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CVIG
CVIG	(Catalog of Very Isolated Galaxies)
*****	Avoid the usage of CVIG, prefer [ATL2005]
Origin	of the Acronym: L (2006KFNT...22..187I)
Details on Acronym: [CVJ2005]
[CVJ2005]	(Cabanac+Valls-Gabaud+Jaunsen+, 2005)
Write:	<<[CVJ2005] For J0332-3557 Lens>> <<[CVJ2005] For J0332-3557 Lensed source>> <<[CVJ2005] For J0332-3557 Einstein Ring>>
N:	3
Object:	G + Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Stat:	is completely incorporated in Simbad
Note:	ESO/VLT/La Silla observations. Discovery of a partial Einstein Ring produced by a massive elliptical galaxy in Fornax Cluster.
in source:	NAME Fornax Cluster
Ref:	=2005A&A...436L..21C
by	CABANAC R.A. , VALLS-GABAUD D., JAUNSEN A.O., LIDMAN C., JERJEN H.
	Astron. Astrophys., 436, 21-25 (2005)
	Discovery of a high-redshift Einstein ring.
o	Text: <[CVJ2005] For J0332-3557 Lens> N=1, <[CVJ2005] For J0332-3557 Lensed source> N=1, <[CVJ2005] For J0332-3557 Einstein Ring> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CVJ99]
[CVJ99]	(Chatzichristou+Vanderriest+Jaffe, 1999) (Not yet in Simbad)
Write:	<<[CVJ99] Cloud N>>
N:	6
Object:	Cloud (SIMBAD class: Cloud)
Note:	Study of the region of 3C 48.
Ref:	=1999A&A...343..407C
by	CHATZICHRISTOU E.T. , VANDERRIEST C., JAFFE W.
	Astron. Astrophys., 343, 407-419 (1999)
	Spectroscopic mapping of the quasar 3C 48 at sub-arcsec resolution.
o	<[CVJ99] Cloud N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CVL2009]
[CVL2009]	(Croxall+van Zee+Lee+, 2009)
Write:	<<[CVL2009] UGC NNNN-NN>> <<[CVL2009] KDG 61-N>> <<[CVL2009] Garland-NN>>
N:	58
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Gemini-North GMOS observations of 10 dwarf galaxies in the M81 group.
in source:	UGC 4305
in source:	UGC 4459
in source:	UGC 5139
in source:	UGC 5336
in source:	UGC 5666
in source:	UGC 5692
in source:	UGC 5918
in source:	UGC 8201
in source:	K68 61
in source:	NAME Garland
Ref:	=2009ApJ...705..723C
by	CROXALL K.V. , VAN ZEE L., LEE H., SKILLMAN E.D., LEE J.C., COTE S., KENNICUTT R.C., MILLER B.W.
	Astrophys. J., 705, 723-738 (2009)
	Chemical abundances of seven irregular and three tidal dwarf galaxies in the M81 group.
o	Table 2: <[CVL2009] UGC 4305-NN> N=9 among (Nos 2-13), <[CVL2009] UGC 4459-N> N=6 among (Nos 2-7), <[CVL2009] UGC 5139-N> N=3 among (Nos 1-5), <[CVL2009] UGC 5336-NN> N=6 among (Nos 3-12), <[CVL2009] UGC 5666-NN> N=11 among (Nos 1-14), <[CVL2009] UGC 5692-N> N=5 among (Nos 3-8), <[CVL2009] UGC 5918-N> (Nos 3-4), <[CVL2009] UGC 8201-NN> N=5 among (Nos 4-15), <[CVL2009] KDG 61-N> (Nos 8-9), <[CVL2009] Garland-NN> N=9 among (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CVL98]
[CVL98]	(Chatzichristou+Vanderriest+Lehnert, 1998) (Not yet in Simbad)
Write:	<<[CVL98] Mkn 789 Aw>> <<[CVL98] Mkn 789 Star N>> <<[CVL98] UGC 4085 Knot A>> <<[CVL98] UGC 4085 Knot N>> <<[CVL98] UGC 4085 Star N>>
N:	8+7
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Tables 2, 3: N=4 regions (Nos A-D) in Mkn 789, region C been subdivided into 'Ce' and 'Cs'. Table 2: N=2 stars in the field of Mkn 789 (Nos 1-2) Table 4: N=2 Knots (Nos A-B), and N=3 Knots (Nos 1-3) in UGC 4085 N=2 stars in the field of UGC 4085 (Nos 1-2)
in source:	Mrk 789
in source:	UGC 4085
Ref:	=1998A&A...330..841C
by	CHATZICHRISTOU E.T. , VANDERRIEST C., LEHNERT M.
	Astron. Astrophys., 330, 841-872 (1998)
	Bidimensional spectroscopy of double galaxies. II. Mkn 789, UGC 4085, UGC 3995.
o	Table 2: <[CVL98] Mkn 789 A> (Nos A-D), <[CVL98] Mkn 789 Star N> (Nos 1-2). Table 3: <[CVL98] Mkn 789 Cw> (Nos Ce, Cs). Table 4: <[CVL98] UGC 4085 Knot A> (Nos A-B), <[CVL98] UGC 4085 Knot N> (Nos 1-3), <[CVL98] UGC 4085 Star N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CVMP
CVMP	(Corradi+Villaver+Mampaso+Perinotto)
Write:	<<CVMP N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Ref:	=1997A&A...324..276C
by	CORRADI R.L.M. , VILLAVER E., MAMPASO A., PERINOTTO M.
	Astron. Astrophys., 324, 276-280 (1997)
	A new, evolved bipolar planetary nebula.
o	<CVMP N> (No. 1).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CVS2005]
[CVS2005]	(Cabanac+Vanzi+Sauvage, 2006)
Write:	<<[CVS2005] LNa>>
N:	12
Object:	(Near IR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Stat:	is completely incorporated in Simbad
Note:	ISAAC ESO VLT observations of the galaxy Hen 2-10 with NAOS-CONICA and ISAAC: N=12 bright L' emitting regions. Complementary archival HST WFPC2 and ISAAC observations, plus VLT NACO, GEMINI OSCIR and VLA observations.
in source:	Hen 2-10
Ref:	=2005ApJ...631..252C
by	CABANAC R.A. , VANZI L., SAUVAGE M.
	Astrophys. J., 631, 252-261 (2005)
	A fresh view of Henize 2-10 with VLT NAOS-CONICA.
o	Fig.2b: Region A, B, C = [VC92] He 2-10 A, B, C, sources NN among (Nos 4-27) not identified. Fig.4: Knots N = [KJ99] Knot N.
o	Fig.2, Table 1: <[CVS2005] LNa> (Nos L1-L2, L3a-L3b, L4a-L4d, L5-L8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CVS97]
[CVS97]	(Chavushyan+Vlasyuk+Stepanian+, 1997)
Write:	<<[CVS97] A>> <<[CVS97] WW>>
N:	2+2
Object:	Component (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Fig.1, Table 1: The gravitational lensed system SBSG 1520+530 has 2 components A and B, and 2 components NW and SE. See also [CSB98], [FCK2002].
in source:	SBSG 1520+530
Ref:	=1997A&A...318L..67C
by	CHAVUSHYAN V.H. , VLASYUK V.V., STEPANIAN J.A., ERASTOVA L.K.
	Astron. Astrophys., 318, 67-70 (1997)
	SBS 1520+530: a new gravitationally lensed system at z=1.855.
o	SBS 1520+530 = SBSG 1520+530 in SIMBAD
o	Fig.1: <[CVS97] A> (Nos A-B). Table 1: <[CVS97] WW> (Nos NW, SE).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CVSO
CVSO	(CIDA Variability Survey in Ori)
Write:	<<CVSO NNNN>> <<CVSO NNNN-N>> <<CVSO NNNNWW>> <<CVSO NNNNW_W>> (not recognised by Simbad, but found in literature)
N:	2057+3+2
Object:	TT* (SIMBAD class: TTauri* = T Tauri Star)
Note:	QUEST camera at the Venezuela National Astronomical Observatory (Centro de Investigaciones De Astronomia = CIDA) is used to search for new members of the assoc. Ori OB 1.
in source:	NAME ASS ORI OB 1-
Ref:	=2005AJ....129..907B
by	BRICENO C. , CALVET N., HERNANDEZ J., VIVAS A.K., HARTMANN L., DOWNES J.J., BERLIND P.
	Astron. J., 129, 907-926 (2005)
	The CIDA variability survey of Orion OB1. I. The low-mass population of Ori OB1a and 1b.
o	Grouping of stars around 25 Ori mentioned in abstract later dubbed NAME 25 Ori GROUP.
o	Table 3: <CVSO NNN> (Nos 1-197).
Ref:	=2007ApJ...661.1119B
by	BRICENO C. , HARTMANN L., HERNANDEZ J., CALVET N., VIVAS A.K., FURESZ G., SZENTGYORGYI A.
	Astrophys. J., 661, 1119-1128 (2007)
	25 Orionis: a kinematically distinct 10 Myr old group in Orion OB1a.
o	Table 2: <CVSO NNN> (Nos 198-258) added.
Ref:	=2011A&A...530A..19B
by	BIAZZO K. , RANDICH S., PALLA F., BRICENO C.
	Astron. Astrophys., 530A, 19-19 (2011)
	Elemental abundances of low-mass stars in the young clusters 25 Orionis and λ Orionis.
o	Table 1: <CVSO NNN> (Nos 259-262) added.
o	In ref list Briceno et al. 2005, A&A, 129, 907 is a misprint for Briceno et al. 2005, AJ, 129, 907.
Ref:	=2019AJ....157...85B
by	BRICENO C. , CALVET N., HERNANDEZ J., VIVAS A.K., MATEU C., DOWNES J.J., LOERINCS J., PEREZ-BLANCO A., BERLIND P., ESPAILLAT C., ALLEN L., HARTMANN L., MATEO M., BAILEY III J.I.
	Astron. J., 157, 85-85 (2019)
	The CIDA Variability Survey of Orion OB1 II. Demographics of the young, low-mass stellar populations.
o	Table 3: <CVSO NNNN> N=2057 among (Nos 1-2099), <CVSO NNNN-N> (Nos 2-1, 59-1, 170-1), <CVSO NNNNWW> (Nos 114SW, 114NE).
=E=	Catalogue in electronic form as <J/AJ/129/907/>
=E=	Catalogue in electronic form as <J/ApJ/661/1119/>
=E=	Catalogue in electronic form as <J/AJ/157/85/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CVT2018]
[CVT2018]	(Curtis+Vanderburg+Torres+, 2018)
Write:	<<[CVT2018] NN>>
N:	10
Object:	* (SIMBAD class: Star)
Note:	Keck II NIRC2, UKIRT WFCAM, and CFHT observations of N=10 stars in the field of K2-231 in the open cluster Ruprecht 147.
in source:	Cl Ruprecht 147
Ref:	=2018AJ....155..173C
by	CURTIS J.L. , VANDERBURG A., TORRES G., KRAUS A.L., HUBER D., MANN A.W., RIZZUTO A.C., ISAACSON H., HOWARD A.W., HENZE C.E., FULTON B.J., WRIGHT J.T.
	Astron. J., 155, 173-173 (2018)
	K2-231 b: a sub-Neptune exoplanet transiting a solar twin in Ruprecht 147.
o	In keywords, EPIC 21980081 is a misprint for EPIC 219800881 .
o	Fig. 3, Table 4: <[CVT2018] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CVU2010]
[CVU2010]	(Cardamone+van Dokkum+Urry+, 2010)
Write:	<<[CVU2010] NNNNN>>
N:	84402
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Subaru 18-band optical medium-band photometry of the Extended Chandra Deep Field-South, as part of the MUSYC survey. Use of Spitzer IRAC data (cf. [TFV2009], and also the SIMPLE survey).
in source:	NAME ECDFS
Ref:	=2010ApJS..189..270C
by	CARDAMONE C.N. , VAN DOKKUM P.G., URRY C.M., TANIGUCHI Y., GAWISER E., BRAMMER G., TAYLOR E., DAMEN M., TREISTER E., COBB B.E., BOND N., SCHAWINSKI K., LIRA P., MURAYAMA T., SAITO T., SUMIKAWA K.
	Astrophys. J., Suppl. Ser., 189, 270-285 (2010)
	The Multiwavelength Survey by Yale-Chile (MUSYC): deep medium-band optical imaging and high-quality 32-band photometric redshifts in the ECDF-S.
o	bvrdetv1, photomv1: <[CVU2010] NNNNN> (Nos 0-84401).
=E=	Catalogue in electronic form as J/ApJS/189/270
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CVV84]
[CVV84]	(Cristiani+Veron-Cetty+Veron, 1984)= (C)
Write:	<<[CVV84] NN>>
N:	75
Object:	QSO (SIMBAD class: QSO = Quasar)
Ref:	=1984A&A...135..122C
by	CRISTIANI S. , VERON-CETTY M.-P., VERON P.
	Astron. Astrophys., 135, 122-128 (1984)
	The completeness of the Braccesi deep quasar survey.
o	Table 3: <[CVV84] NN> (Nos 1-75)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CW
CW	(C. Wilson)
Write:	<<CW Blue NNN>> <<CW Red NN>> <<CW Assoc NN>>
N:	268+77+13
Object:	* + Assoc. (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=268 blue stars, format 'Blue NNN' Table 2: N= 77 red stars, format 'Red NN' Table 4: N=13 assoc. format 'Ass NN'
in source:	NGC 6822
Ref:	=1992AJ....104.1374W
by	WILSON C.D.
	Astron. J., 104, 1374-1394 (1992)
	The stellar populations of NGC 6822.
o	(Erratum) Erratum A.J. 109, p. 449-451
o	Identifications: T. 4: Hubble R = [H25] R, Ho = [H77] HII NN, HK = [HKL88]. text p. 1389: Hodge-OB = [H77] Ass NN, text p. 1392: CNN = [H77] Cl* NN. Corrected coordinates for tables 1 and 2 in the erratum.
o	Table 1: <CW Blue NNN> (Nos 1-268), Table 2: <CW Red NN> (Nos 1-77), Table 4: <CW Ass NN> (Nos 1-13)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CW
CW	(Cartwheel galaxy)
*****	Avoid the usage of CW, prefer [H95]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CW
CW	(Case univ., Western reserve)
Write:	<<NAME CW HHMM+DDd>>
N:	1
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Survey of the North Galactic Pole region, in a search for emission-line galaxies, in preparation. Rounded, not truncated coord. N=1, CW 1103+254
Ref:	=1982PASP...94..682S
by	SHORE S.N. , FOLTZ C.B., WASILEWSKI A.J., BYARD P.L., WAGNER R.M.
	Publ. Astron. Soc. Pac., 94, 682-689 (1982)
	CW 1103+254 : a new cataclysmic at high galactic latitude.
o	<NAME CW 1103+254>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CW2007]
[CW2007]	(Cao+Wu, 2007)
Write:	<<[CW2007] YSCC>> <<[CW2007] KN>> <<[CW2007] YSCC N>> <<[CW2007] KN N>>
N:	1+3+5+2+3
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	Search for Young Stellar Cluster Complexes (YSCC) and stellar clusters in APG 24. Use of archival HST, SDSS, GALEX, and Spitzer data.
in source:	APG 24
Ref:	=2007AJ....133.1710C
by	CAO C. , WU H.
	Astron. J., 133, 1710-1721 (2007)
	Multiwavelength study of young massive star clusters in the interacting galaxy Arp 24.
o	Table 1: <[CW2007] YSCC> N=1, <[CW2007] KN> (Nos K1-K3). Table 2: <[CW2007] YSCC N> (Nos 1-5), <[CW2007] K2 N> (Nos 1-2), <[CW2007] K3 N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CW2008]
[CW2008]	(Chen Wright, 2008)
Write:	<<[CW2008] JHHMMSS+DDMMSS>>
N:	64
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Search for point sources in the WMAP 3yr data. +N=64 sources, among which N=21 are not in the WMAP JHHMMDDMM catalog.
Ref:	=2008ApJ...681..747C
by	CHEN X. , WRIGHT E.L.
	Astrophys. J., 681, 747-755 (2008)
	Extragalactic point-source search in WMAP 61 and 94 GHz data.
o	Table 1: <[CW2008] JHHMMSS+DDMMSS> N=64.
=E=	Catalogue in electronic form as <J/ApJ/681/747/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CW2009]
[CW2009]	(Chomiuk+Wilcots, 2009)= ([CW2009a])
Write:	<<[CW2009] NNNNN-NN>>
N:	46+29+24+30
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Use of archival VLA 3.6, 6, and 20cm observations to search for discrete sources in N=4 Irr galaxies.
in source:	NGC 1569
in source:	NGC 4214
in source:	NGC 2366
in source:	NGC 4449
Ref:	=2009AJ....137.3869C
by	CHOMIUK L. , WILCOTS E.M.
	Astron. J., 137, 3869-3883 (2009)
	A search for radio supernova remnants in four irregular galaxies.
o	Table 4: <[CW2009] N1569-NN> (Nos 01-46). Table 5: <[CW2009] N4214-NN> (Nos 01-29). Table 6: <[CW2009] N2366-NN> (Nos 01-24). Table 7: <[CW2009] N4449-NN> (Nos 01-30).
=E=	Catalogue in electronic form as <J/AJ/137/3869/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CW2009a]
[CW2009a]	(Chomiuk+Wilcots, 2009)
*****	Avoid the usage of [CW2009a], prefer [CW2009]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CW2009b]
[CW2009b]	(Chen+Wright, 2009)
Write:	<<[CW2009b] WMAP JHHMMSS+DDMM>>
N:	368+14
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Extragalactic point source search using the five-year Wilkinson Microwave Anisotropy Probe (WMAP) 41, 61, and 94GHz (Q, V, and W bands) temperature maps. See also WMAP.
Ref:	=2009ApJ...694..222C
by	CHEN X. , WRIGHT E.L.
	Astrophys. J., 694, 222-234 (2009)
	Extragalactic point source search in five-year WMAP 41, 61, and 94 Ghz maps.
o	Tables 1,2: <[CW2009b] WMAP JHHMMSS+DDMM> N=368+14.
=E=	Catalogue in electronic form as <J/ApJ/694/222/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CW83]
[CW83]	(Carnochan+Wilson, 1983)= (UV) = (UVO)
Write:	<<[CW83] HHMM+DD>>
N:	13
Object:	UV Obj. (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	Sky Survey Telescope S2/S6 aboard TD1
Ref:	=1983MNRAS.202..317C
by	CARNOCHAN D.J. , WILSON R.
	Mon. Not. R. Astron. Soc., 202, 317-345 (1983)
	A survey of ultraviolet objects.
o	<[CW83] HHMM+DD> N=13
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CW84]
[CW84]	(CHini+Wink, 1984) (Not yet in Simbad)
Write:	<<[CW84] SNNN-N>>
N:	34
Object:	* (SIMBAD class: Star)
Note:	N=34 stars in N=17 Sh 2-NNN HII regions.
Ref:	=1984A&A...139L...5C
by	CHINI R. , WINK J.E.
	Astron. Astrophys., 139, 5-8 (1984)
	The galactic rotation outside the solar circle.
o	Table 1: <[CW84] SNNN-N> N=34.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CW93]
[CW93]	(Cunow+Wargau, 1993)
Write:	<<[CW93] ACO NNNN NN>> <<[CW93] ACO S NNN NN>>
N:	145
Object:	G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 3: format 'ACO 2810 NN', N=19 Table 4: format 'ACO S 133 NN', N=10 Table 5: format 'ACO 3106 NN', N=22 Table 6: format 'ACO S 463 NN', N=10 Table 7: format 'ACO 3279 NN', N=32 Table 8: format 'ACO 514 NN', N=36 Table 9: format 'ACO 3341 NN', N=16
Ref:	=1993A&AS..102..331C
by	CUNOW B. , WARGAU W.F.
	Astron. Astrophys., Suppl. Ser., 102, 331-338 (1993)
	Photometric CCD sequences for calibration of the ESO(R) survey.
o	Table 8: ACO 514 not O0514
o	Table 3: <[CW93] ACO 2810 NN> N=19. Table 4: <[CW93] ACO S 133 NN> N=10. Table 5: <[CW93] ACO 3106 NN> N=22. Table 6: <[CW93] ACO S 433 NN> N=10. Table 7: <[CW93] ACO 3279 NN> N=32. Table 8: <[CW93] ACO 514 NN> N=36. Table 9: <[CW93] ACO 3341 NN> N=16
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CW94]
[CW94]	(Cunow+Wargau, 1994)= ([CW94a])
Write:	<<[CW94] ACO NNNN NN>> <<[CW94] ACO S 191 NN>>
N:	183
Object:	G + * in ClG (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 3: format 'ACO 2841 NN', N=18 Table 4: format 'ACO S 191 NN', N=21 Table 5: format 'ACO 3103 NN', N=26 Table 6: format 'ACO 495 NN', N=30 Table 7: format 'ACO 3888 NN', N=28 Table 8: format 'ACO 2583 NN', N=29 Table 9: format 'ACO 4028 NN', N=31.
in source:	ACO 2841
in source:	ACO S 191
in source:	ACO 3103
in source:	ACO 495
in source:	ACO 3888
in source:	ACO 2583
in source:	ACO 4028
Ref:	=1994A&AS..107..277C
by	CUNOW B. , WARGAU W.F.
	Astron. Astrophys., Suppl. Ser., 107, 277-283 (1994)
	Photometric CCD sequences in 7 southern Abell clusters.
o	Tables 3 to 9: <[CW94] ACO NNNN NN> or <[CW94] ACO S NNN NN> N=183
=E=	Catalogue in electronic form as J/A+AS/107/277
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CW94a]
[CW94a]	(Cunow+Wargau, 1994) (Not yet in Simbad)
*****	Avoid the usage of [CW94a], prefer [CW94]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CW94b]
[CW94b]	(Cesaroni+Wilson, 1994)= (ON) = (OS)
Write:	<<[CW94b] ON N>> <<[CW94b] OS N>>
N:	5+7
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Table 1: 5 ammonia clumps in Orion-North, format 'ON N' and 7 ammonia clumps in Orion-South, format 'OS N'
in source:	NAME Orion Nebula
Ref:	=1994A&A...281..209C
by	CESARONI R. , WILSON T.L.
	Astron. Astrophys., 281, 209-219 (1994)
	An ammonia study of the Orion streamer.
o	<[CW94b] ON N> N=5, <[CW94b] OS N> N=7
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CW95]
[CW95]	(Conway+Wrobel, 1995)
Write:	<<[CW95] A>>
N:	6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
in source:	Mrk 501
Ref:	=1995ApJ...439...98C
by	CONWAY J.E. , WROBEL J.M.
	Astrophys. J., 439, 98-112 (1995)
	A helical jet in the orthogonally misaligned BL Lacertae object Markarian 501 (B1652+398).
o	Figs 2, 3: <[CW95] A> (Nos A-F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CW97]
[CW97]	(Chandler+Wood, 1997)
Write:	<<[CW97] N>>
N:	6
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
in source:	[RLK73] IRc 2
Ref:	=1997MNRAS.287..445C
by	CHANDLER C.J. , WOOD D.O.S.
	Mon. Not. R. Astron. Soc., 287, 445-454 (1997)
	VLA observations of 43-GHz continuum and CS J = 1-0 emission from Orion-IRc2 and the hot core.
o	Table 1: <[CW97] N> (Nos 1-6)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CW98]
[CW98]	(Chini+Wargau, 1998)= (IRS)
Write:	<<[CW98] IRS NNW>>
N:	37+1
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	M 17 = NGC 6618
Ref:	=1998A&A...329..161C
by	CHINI R. , WARGAU W.F.
	Astron. Astrophys., 329, 161-168 (1998)
	Young stellar objects and abnormal extinction within M17.
o	CEN = Cl* NGC 6618 CEN in SIMBAD
o	Table 2: <[CW98] IRS NN> (Nos 1-37)
Ref:	=2000A&A...357L..33C
by	CHINI R. , NIELBOCK M., BECK R.
	Astron. Astrophys., 357, 33-36 (2000)
	The birth of massive twins in M 17.
o	Table 1: <[CW98] IRS 5S> added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWA2006]
[CWA2006]	(Cannon+Walter+Armus+, 2006)
Write:	<<[CWA2006] NGC 6822 NN>>
N:	16
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Spitzer MIPS and IRAC observations of NGC 6822.
in source:	NGC 6822
Ref:	=2006ApJ...652.1170C
by	CANNON J.M. , WALTER F., ARMUS L., BENDO G.J., CALZETTI D., DRAINE B.T., ENGELBRACHT C.W., HELOU G., KENNICUTT R.C.Jr, LEITHERER C., ROUSSEL H., BOT C., BUCKALEW B.A., DALE D.A., DE BLOK W.J.G., GORDON K.D., HOLLENBACH D.J., JARRETT T.H., MEYER M.J., MURPHY E.J., SHETH K., THORNLEY M.D.
	Astrophys. J., 652, 1170-1187 (2006)
	The nature of infrared emission in the Local Group dwarf galaxy NGC 6822 as revealed by Spitzer.
o	Table 1: <[CWA2006] NGC 6822 NN> (Nos 1-16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CWAT
CWAT	(COSMOS, Wide Angle Tail)
Write:	<<CWAT N>>
N:	2
Object:	rG (SIMBAD class: RadioG = Radio Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Identification of a complex galaxy cluster in the COSMOS Field via a Wide Angle Tail radio galaxy.
in source:	COSMOS Field:NAME CWAT-01 Parent Cluster = NAME CWAT-01 Parent Cluster
Ref:	=2007ApJS..172..295S
by	SMOLCIC V. , SCHINNERER E., FINOGUENOV A., SAKELLIOU I., CARILLI C.L., BOTZLER C.S., BRUSA M., SCOVILLE N., AJIKI M., CAPAK P., GUZZO L., HASINGER G., IMPEY C., JAHNKE K., KARTALTEPE J.S., McCRACKEN H.J., MOBASHER B., MURAYAMA T., SASAKI S.S., SHIOYA Y., TANIGUCHI Y., TRUMP J.R.
	Astrophys. J., Suppl. Ser., 172, 295-313 (2007)
	A wide-angle tail radio galaxy in the COSMOS field: evidence for cluster formation.
o	<CWAT N> (No. 1).
Ref:	=2011MmSAI..82..161O
by	OKLOPCIC A. , SMOLCIC V., GIODINI S., ZAMORANI G., BIRZAN L., SCHINNERER E., CARILLI C.L., FINOGUENOV A., LILLY S., KOEKEMOER A., SCOVILLE N.Z.
	MmSAI, 82, 161-164 (2011)
	A wide-angle tail galaxy at z = 0.53 in the COSMOS field.
o	<CWAT N> (No. 2) added.
o	Galaxy at z = 0.53 in the title is CWAT 2 in SIMBAD
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CWB2004]
[CWB2004]	(Carilli+Walter+Bertoldi+, 2004)
Write:	<<[CWB2004] J1148+5251 N>>
N:	5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA images of radio-sources brighter than 22mJy with 8' of QSO J1148+5251.
Ref:	=2004AJ....128..997C
by	CARILLI C.L. , WALTER F., BERTOLDI F., MENTEN K.M., FAN X., LEWIS G.F., STRAUSS M.A., COX P., BEELEN A., OMONT A., MOHAN N.
	Astron. J., 128, 997-1001 (2004)
	Radio continuum imaging of Far-Infrared-Luminous QSOs at z > 6.
o	Fig.2, Table 2: <[CWB2004] J1148+5251 N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWB2005]
[CWB2005]	(Cannon+Walter+Bendo+, 2005)= (SGS)
Write:	<<[CWB2005] SGS N>>
N:	6
Object:	Super Giant Shell (SIMBAD class: HIshell = Interstellar Shell)
Stat:	is completely incorporated in Simbad
Note:	Resolved Spitzer Space Telescope imaging of the Super Giant Shell region of IC 2574: the whole SGS is divided in 6 sub-regions.
in source:	IC 2574:NAME IC 2574 SGS = NAME IC 2574 SGS
Ref:	=2005ApJ...630L..37C
by	CANNON J.M. , WALTER F., BENDO G.J., CALZETTI D., DALE D.A., DRAINE B.T., ENGELBRACHT C.W., GORDON K.D., HELOU G., KENNICUTT R.C.Jr, MURPHY E.J., THORNLEY M.D., ARMUS L., HOLLENBACH D.J., LEITHERER C., REGAN M.W., ROUSSEL H., SHETH K.
	Astrophys. J., 630, 37-40 (2005)
	Spitzer observations of the supergiant shell region in IC 2574.
o	Table 1: <[CWB2005] SGS N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWB2011]
[CWB2011]	(Crawford+Wirth+Bershady+, 2011)= (WLTV)
Write:	<<[CWB2011] WLTV JHHMMSS.ss+DDMMSS.s>>
N:	1286
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Keck II DEIMOS spectroscopy of N=1286 sources pre-selected on imaging data from the WYIN telescope, in the frame of the WIYN Long-Term Variability survey (WLTV).
in source:	ClG 0451-0305 = 1E 0451.6-0305
in source:	ClG 0016+1609 = 1E 0015.9+1609
in source:	ClG J1324+3011
in source:	ClG 1054-0321 = 1E 1054.4-0321
in source:	ClG 1603+4313
Ref:	=2011ApJ...741...98C
by	CRAWFORD S.M. , WIRTH G.D., BERSHADY M.A., HON K.
	Astrophys. J., 741, 98 (2011)
	Spectroscopy of luminous compact blue galaxies in distant clusters. I. Spectroscopic data.
o	Table 4: <[CWB2011] WLTV JHHMMSS.ss+DDMMSS.s> N=1286.
=E=	Catalogue in electronic form as J/ApJ/741/98
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWB94]
[CWB94]	(Colbert+Wilson+Bland-Hawthorn, 1994)
Write:	<<[CWB94] N>> <<[CWB94] NN>> <<[CWB94] WN>> <<[CWB94] WW>> <<[CWB94] Nd>>
N:	18
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA map of NGC 6240. The nuclear region is designated 'N', with 3 sources (Nos N1-N3), a diffuse nuclear region 'Nd', and a southern source 'S'. The Western Arm is designated 'W', with clumps (Nos W0-W4). Other radio components are found later: (S1, S2, E1, NW, NE, SE).
in source:	NGC 6240
Ref:	=1994ApJ...436...89C
by	COLBERT E.J.M. , WILSON A.S., BLAND-HAWTHORN J.
	Astrophys. J., 436, 89-101 (1994)
	The radio emission from the ultraluminous far-infrared galaxy NGC 6240.
o	N1* and N2*, unresolved components of N1 and N2, not in SIMBAD.
o	Figs 2, 3, Table 3: <[CWB94] AN> (Nos N, N1-N3), <[CWB94] WN> (Nos S, W, W1-W4), <[CWB94] Ad> (No. Nd).
Ref:	=2004AJ....127..239G
by	GALLIMORE J.F. , BESWICK R.
	Astron. J., 127, 239-251 (2004)
	Parsec-scale radio structure of the double active nucleus of NGC 6240.
o	Par. 2.1: the candidate radio supernova is [G2000] J165258.8998+022403.591, later designated as [CWB94] S2.
o	<[CWB94] WN> (No. S1) added.
Ref:	=2007ApJ...659..283I
by	IONO D. , WILSON C.D., TAKAKUWA S., YUN M.S., PETITPAS G.R., PECK A.B., HO P.T.P., MATSUSHITA S., PIHLSTROM Y.M., WANG Z.
	Astrophys. J., 659, 283-295 (2007)
	High-resolution imaging of warm and dense molecular gas in the nuclear region of the luminous infrared galaxy NGC 6240.
o	2 QSOs not identified : 1743-038 and 1549+026
o	<[CWB94] WN> (No. S2) added.
Ref:	=2007ApJ...661..173B
by	BAAN W.A. , HAGIWARA Y., HOFNER P.
	Astrophys. J., 661, 173-184 (2007)
	H I and OH absorption toward NGC 6240.
o	Table 1: <[CWB94] WN> (Nos W0, E1) added, <[CWB94] WW> (Nos NW, NE, SE).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWB95]
[CWB95]	(Carballo+Warwick+Barcons+, 1995)
Write:	<<[CWB95] NHNN>> <<[CWB95] AHNN>> <<[CWB95] BHNN>> <<[CWB95] JHHMMSS.s+DDMMSS>>
N:	51+64
Object:	(X) + * (SIMBAD class: X = X-ray Source)
Note:	ROSAT PSPC observations. The X-ray sources are labelled by the authors with the formats 'NHNN' or 'AHNN' where the first digit stands for the survey field identifier (1, 2, 3, 4, 5, 6, A or B) followed by the letter 'H' (reflecting that the source search was performed in the Hard band) and the number 'NN' assigned to the source. The optical objects in the X-ray error circle have no format assigned by the authors, so we give them a 2000 eq. coordinates format: JHHMMSS.s+DDMMSS Table 2: N=9 X-ray sources, N=11 * Table 3: N=16 X-ray sources, N=26 G Table 5: N=26 X-ray sources, N=27 QSO
Ref:	=1995MNRAS.277.1312C
by	CARBALLO R. , WARWICK R.S., BARCONS X., GONZALEZ-SERRANO J.I., BARBER C.R., MARTINEZ-GONZALEZ E., PEREZ-FOURNON I., BURGOS J.
	Mon. Not. R. Astron. Soc., 277, 1312-1326 (1995)
	The ROSAT UK Medium Sensitivity Survey: optical identification and relation to X-ray spectral properties.
o	Tables 2, 3, 5: <[CWB95] NHNN> or <[CWB95] AHNN> N=51, <[CWB95] JHHMMSS.s+DDMMSS> N=64
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWB96]
[CWB96]	(Clocchiatti+Wheeler+Benetti+, 1996)
Write:	<<[CWB96] NN>>
N:	21
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Chart Photometric sequence around SN 1983N
Ref:	=1996ApJ...459..547C
by	CLOCCHIATTI A. , WHEELER J.C., BENETTI S., FRUEH M.
	Astrophys. J., 459, 547-554 (1996)
	SN 1983N and the nature of stripped envelope-core collapse supernovae.
o	cross-id. 'H' p. 549 not in SIMBAD
o	Table 2: <[CWB96] NN> (Nos 1-21)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWC2013]
[CWC2013]	(Chapman +Widrow+Collins+, 2013)
Write:	<<[CWC2013] And XXII NNN>> <<[CWC2013] ECN NNN>>
N:	13+3
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Keck II DEIMOS observations of candidate member stars of the dwarf spheroidal galaxy And XXII and the two extended clusters NAME M33-EC1 and NAME M33-EC2.
in source:	And XXII
in source:	NAME M33-EC1
in source:	NAME M33-EC2
Ref:	=2013MNRAS.430...37C
by	CHAPMAN S.C. , WIDROW L., COLLINS M.L.M., DUBINSKI J., IBATA R.A., RICH M., FERGUSON A.M.N., IRWIN M.J., LEWIS G.F., MARTIN N., McCONNACHIE A., PENARRUBIA J., TANVIR N.
	Mon. Not. R. Astron. Soc., 430, 37-49 (2013)
	Dynamics in the satellite system of Triangulum: is And XXII a dwarf satellite of M33 ?
o	Table 2: <[CWC2013] And XXII NNN> N=13 among (Nos 6-131). Table 3: <[CWC2013] ECN NNN> (Nos EC1 20, EC1 127, EC2 70).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWD2016]
[CWD2016]	(Chandar+Whitmore+Dinino+, 2016)
Write:	<<[CWD2016] NNNN>>
N:	3812
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST WFPC2 observations of N=3812 star clusters in M51. Use of archival HST ACS and WFPC2 data.
in source:	NGC 5194 = M 51
Ref:	=2016ApJ...824...71C
by	CHANDAR R. , WHITMORE B.C., DININO D., KENNICUTT R.C., CHIEN L.-H., SCHINNERER E., MEIDT S.
	Astrophys. J., 824, 71-71 (2016)
	The age, mass, and size distributions of star clusters in M51.
o	Table 1: <[CWD2016] NNNN> (Nos 1-3812).
=E=	Catalogue in electronic form as <J/ApJ/824/71/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWD95]
[CWD95]	(Cecil+Wilson+De Pree, 1995)
Write:	<<[CWD95] N>>
N:	9
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI and PSPC observations.
in source:	NGC 4258
Ref:	=1995ApJ...440..181C
by	CECIL G. , WILSON A.S., DE PREE C.
	Astrophys. J., 440, 181-190 (1995)
	Hot shocked gas along the jets of NGC 4258 (M 106).
o	<[CWD95] N> N=9
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWD97]
[CWD97]	(Corbel+Wallyn+Dame+, 1997)
Write:	<<[CWD97] MC+VVA>>
N:	10+2
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	SEST 12CO(1-0) observations of 'NAME SGR 1806-20'. Deetection of several molecular clouds. In the format 'VV' stands for the V(LSR) velocity. MC 13 is resolved in 2004 into two components designated as 13A and 13B.
Ref:	=1997ApJ...478..624C
by	CORBEL S. , WALLYN P., DAME T.M., DUROUCHOUX P., MAHONEY W.A., VILHU O., GRINDLAY J.E.
	Astrophys. J., 478, 624-630 (1997)
	The distance of the soft γ repeater SGR 1806-20.
o	Text: <[CWD97] MC+VV> N=7.
Ref:	=2004A&A...419..191C
by	CORBEL S. , EIKENBERRY S.S.
	Astron. Astrophys., 419, 191-201 (2004)
	The connection between W31, SGR 1806-20, and LBV 1806-20: Distance, extinction, and structure.
o	Table 1: <[CWD97] MC+VVA> N=3+2 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWF2012]
[CWF2012]	(Connelly+Wilman+Finoguenov+, 2012)
Write:	<<[CWF2012] DDD.dddddd+DD.dddddd>> <<[CWF2012] XRHHhNN>> <<[CWF2012] OPHHhNNN>>
N:	4702+67+38
Object:	G + Group of G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Two samples of galaxy groups (in two CNOC2 fields, RA14h and RA21h), containing N=67 high-quality X-ray-selected systems and N=38 optically (spectroscopically) selected systems. VLT FORS2, Magellan IMACS, and Gemini GMOS follow-up spectroscopy of N=4704 sources.
Ref:	=2012ApJ...756..139C
by	CONNELLY J.L. , WILMAN D.J., FINOGUENOV A., HOU A., MULCHAEY J.S., McGEE S.L., BALOGH M.L., PARKER L.C., SAGLIA R., HENDERSON R.D.E., BOWER R.G.
	Astrophys. J., 756, 139 (2012)
	Exploring the diversity of groups at 0.1 < z < 0.8 with X-ray and optically selected samples.
o	Table 2: <[CWF2012] DDD.dddddd+DD.dddddd> N=4702. Tables 3-4+7: <[CWF2012] XRHHhNN> N=67 among (Nos XR14h01-XR14h47, XR21h06-XR21h69). Tables 5-6+8: <[CWF2012] OPHHhNNN> N=38 among (Nos OP14h01-OP14h40, OP21h101-OP21h140).
=E=	Catalogue in electronic form as <J/ApJ/756/139/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWF94]
[CWF94]	(Cote+Welch+Fischer+, 1994)
Write:	<<[CWF94] NNN>>
N:	879
Object:	* (SIMBAD class: Star)
Note:	Table 4: NGC 3201 field stars, acronym '[CWF94] NNN'. Table 2: 'CL* NGC 3201 CWFD VNN' N=19. Table 3: 'CL* NGC 3201 CWFD 3-NNN' N=420.
in source:	NGC 3201
Ref:	=1994ApJS...90...83C
by	COTE P. , WELCH D.L., FISCHER P., DA COSTA G.S., TAMBLYN P., SEITZER P., IRWIN M.J.
	Astrophys. J., Suppl. Ser., 90, 83-113 (1994)
	A search for binaries in the globular cluster NGC 3201.
o	Table 2: <CL* NGC 3201 CWFD VNN> (Nos V1-V19). Table 3: <CL* NGC 3201 CWFD 3-NNN> (Nos 3-1 to 3-420). Table 4: <[CWF94] NNN> (Nos 1-879).
=E=	Catalogue in electronic form as J/ApJS/90/83
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWG2001]
[CWG2001]	(Croom+Warren+Glazebrook, 2001)
Write:	<<[CWG2001] KX NN>> <<[CWG2001] UVX N>> <<[CWG2001] KG NN>>
N:	54+2+16
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	ESO EIS observations of the Chandra Deep Field South. In the format 'KX' stands for K-excess survey, 'UVX' for UVX candidates, 'KG' for K'band galaxies.
in source:	NAME CDFS
Ref:	=2001MNRAS.328..150C
by	CROOM S.M. , WARREN S.J., GLAZEBROOK K.
	Mon. Not. R. Astron. Soc., 328, 150-158 (2001)
	A small-area faint KX redshift survey for QSOs in the ESO Imaging Survey Chandra Deep Field South.
o	Tables 1, 2: <[CWG2001] KXNN> (Nos KX01 to KX54). Table 3: <[CWG2001] UVXN> (Nos UVX1 to UVX2). Table 4: <[CWG2001] KGNN> (Nos KG01 to KG16).
=E=	Catalogue in electronic form as J/MNRAS/328/150
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWG2006]
[CWG2006]	(Chen+Wang+Gotthelf+, 2006)
Write:	<<[CWG2006] N>>
N:	8
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS observations of the field of LHA 120-N 157B in the LMC.
in source:	Magellanic Clouds:LMC:LHA 120-N 157B = LHA 120-N 157B
Ref:	=2006ApJ...651..237C
by	CHEN Y. , WANG Q.D., GOTTHELF E.V., JIANG B., CHU Y.-H., GRUENDL R.
	Astrophys. J., 651, 237-249 (2006)
	Chandra ACIS spectroscopy of N157B: a young composite supernova remnant in a superbubble.
o	Table 2: <[CWG2006] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWH2004]
[CWH2004]	(Clewlwy+Warren+Hewett+, 2004)
Write:	<<[CWH2004] AAAA-NNN>> <<[CWH2004] AAANN-NNN>> <<[CWH2004] AANNN-NNN>>
N:	461+90+4
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	CCD photometry of candidate A-type, blue harizontal-branch, and horizontal branc stars selected from six UKST fields. First part of the formatstands for field with for each field, stars in the complete sample are prefixed 'C', otherwise stars are prefixed 'I'.
Ref:	=2004MNRAS.352..285C
by	CLEWLEY L. , WARREN S.J., HEWETT P.C., NORRIS J.E., EVANS N.W.
	Mon. Not. R. Astron. Soc., 352, 285-298 (2004)
	Distant field blue horizontal branch stars and the mass of the Galaxy - II. Photometry and spectroscopy of UKST candidates 16<B<19.5, 11<R<52kpc.
o	Objects from table 11 ISGP-006, ISA94-075, IMTF-017 and IMTF-034 not id entified.
o	Tables 4, 7, 11: <[CWH2004] AAAA-NNN>, <[CWH2004] AAANN-NNN>, <[CWH2004] AANNN-NNN>, N=461+90+4.
=E=	Catalogue in electronic form as J/MNRAS/352/285
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWH2006]
[CWH2006]	(Cackett+Wijnands+Heinke+, 2006)= (CX)
Write:	<<[CWH2006] CXNN>>
N:	14
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-S observation of the globular cluster Terzan 1.
in source:	Cl Terzan 1
Ref:	=2006MNRAS.369..407C
by	CACKETT E.M. , WIJNANDS R., HEINKE C.O., POOLEY D., LEWIN W.H.G., GRINDLAY J.E., EDMONDS P.D., JONKER P.G., MILLER J.M.
	Mon. Not. R. Astron. Soc., 369, 407-415 (2006)
	A Chandra X-ray observation of the globular cluster Terzan 1.
o	Table 1, col(2): <[CWH2006] CXNN> (Nos CX1-CX14) = Table 1, col(1): <CXOGlb JHHMMSS.s+DDMMSS> N=14.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWH98]
[CWH98]	(Chu+Wei+Hu+, 1998)
Write:	<<[CWH98] JHHMM+DDMM>>
N:	6
Object:	QSO + G (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	N=5 QSO and and N=1 Seyfert G in the field of NGC 3516 Objects from 1997A&A...319...33A are also [A97c] JHHMMSS.s+DDMMSS See [A97c]
in source:	NGC 3516
Ref:	=1998ApJ...500..596C
by	CHU Y. , WEI J., HU J., ZHU X., ARP H.
	Astrophys. J., 500, 596-598 (1998)
	Quasars around the Seyfert galaxy NGC 3516.
o	Table 3: <[CWH98] JHHMM+DDMM> N=6
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWH99]
[CWH99]	(Cao+Wei+Hu, 1999)
Write:	<<[CWH99] JHHMMSS.s+DDMMSS>>
N:	37
Object:	Opt. Id. (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=37 possible optical identifications of N=34 RASS-BSC sources.
Ref:	=1999A&AS..135..243C
by	CAO L. , WEI J.-Y., HU J.-Y.
	Astron. Astrophys., Suppl. Ser., 135, 243-253 (1999)
	High X-ray-to-optical flux ratio RASS-BSC sources. I. The optical identification.
o	Table 1: <[CWH99] JHHMMSS.s+DDMMSS> N=37.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CWISE
CWISE	(CatWISE Catalog)
Write:	<<CWISE JHHMMSS.ss+DDMMSS.s>>
N:	about 1000000000 (SIMBAD class: MidIR = Mid-IR Source (3 to 30 µm))
Note:	CatWISE is a full-sky catalog consisting of sources selected at 3.4 and 4.6 microns from four years of WISE and NEOWISE survey data. CatWISE adapted AllWISE software to detect and measure the sources in unWISE images created from these data. The catalog includes the measured motion of sources over the more than six years spanned by the data. The catalogs and co-added images will be made available via the NASA/IPAC Infrared Science Archive.
Notes:	https://iopscience.iop.org/2515-5172/2/3/140/ (2018RNAAS...2c.140M) CatWISE data overview paper (to be submitted in March) Discovery of a very cool Y dwarf with CatWISE (to be submitted in March) See also CWISEP for the preliminary release.
Ref:	=2021ApJS..253....8M
by	MAROCCO F. , EISENHARDT P.R.M., FOWLER J.W., KIRKPATRICK J.D., MEISNER A.M., SCHLAFLY E.F., STANFORD S.A., GARCIA N., CASELDEN D., CUSHING M.C., CUTRI R.M., FAHERTY J.K., GELINO C.R., GONZALEZ A.H., JARRETT T.H., KOONTZ R., MAINZER A., MARCHESE E.J., MOBASHER B., SCHLEGEL D.J., STERN D., TEPLITZ H.I., WRIGHT E.L.
	Astrophys. J., Suppl. Ser., 253, 8-8 (2021)
	The CatWISE2020 Catalog.
o	<CWISE JHHMMSS.ss+DDMMSS.s> N≃1000000000. <CWISER JHHMMSS.ss+DDMMSS.s> N=111394986. JPL/Caltech
=E=	Catalogue in electronic form as <II/365/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CWISEP
CWISEP	(CatWISE Preliminary Catalog)
Write:	<<CWISEP JHHMMSS.ss+DDMMSS.s>>
N:	about 1000000000 (SIMBAD class: MidIR = Mid-IR Source (3 to 30 µm))
Note:	CatWISE is a full-sky catalog consisting of sources selected at 3.4 and 4.6 microns from four years of WISE and NEOWISE survey data. CatWISE adapted AllWISE software to detect and measure the sources in unWISE images created from these data. The catalog includes the measured motion of sources over the more than six years spanned by the data. The catalogs and co-added images will be made available via the NASA/IPAC Infrared Science Archive.
Notes:	https://iopscience.iop.org/2515-5172/2/3/140/ (2018RNAAS...2c.140M) CatWISE data overview paper (to be submitted in March) Discovery of a very cool Y dwarf with CatWISE (to be submitted in March) This is the initial, preliminary, release, hence the "P" suffix. We anticipate an updated release which will not use the P suffix for the acronym (ie CWISE).
Ref:	=2020ApJS..247...69E
by	EISENHARDT P.R.M. , MAROCCO F., FOWLER J.W., MEISNER A.M., KIRKPATRICK J.D., GARCIA N., JARRETT T.H., KOONTZ R., MARCHESE E.J., STANFORD S.A., CASELDEN D., CUSHING M.C., CUTRI R.M., FAHERTY J.K., GELINO C.R., GONZALEZ A.H., MAINZER A., MOBASHER B., SCHLEGEL D.J., STERN D., TEPLITZ H.I., WRIGHT E.L.
	Astrophys. J., Suppl. Ser., 247, 69-69 (2020)
	The CatWISE Preliminary Catalog: motions from WISE and NEOWISE data.
o	<CWISEP JHHMMSS.ss+DDMMSS.s> N~1000000000. <CWISEPR JHHMMSS.ss+DDMMSS.s> N=111394986. JPL/Caltech
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CWISEPR
CWISEPR	(CatWISE Preliminary Reject file)
Write:	<<CWISEPR JHHMMSS.ss+DDMMSS.s>>
N:	111394986 (SIMBAD class: MidIR = Mid-IR Source (3 to 30 µm))
Note:	CatWISE is a full-sky catalog consisting of sources selected at 3.4 and 4.6 microns from four years of WISE and NEOWISE survey data. The Reject file consists of sources which do NOT satisfy the following criteria: 1) Primary in tile. As in WISE, the area of the sky is divided into 18,240 tiles which have some overlap and hence duplicate source entries. The primary in tile designation means the source is further from the tile edge than are the duplicate entries. 2) Have no identified artifact and SNR ≥ 5 at 3.4 microns, or have no identified artifact and SNR ≥ 5 at 4.6 microns.
Notes:	CatWISE data overview paper (to be submitted in March); Discovery of a very cool Y dwarf with CatWISE (to be submitted in March)
Ref:	=2020ApJS..247...69E
by	EISENHARDT P.R.M. , MAROCCO F., FOWLER J.W., MEISNER A.M., KIRKPATRICK J.D., GARCIA N., JARRETT T.H., KOONTZ R., MARCHESE E.J., STANFORD S.A., CASELDEN D., CUSHING M.C., CUTRI R.M., FAHERTY J.K., GELINO C.R., GONZALEZ A.H., MAINZER A., MOBASHER B., SCHLEGEL D.J., STERN D., TEPLITZ H.I., WRIGHT E.L.
	Astrophys. J., Suppl. Ser., 247, 69-69 (2020)
	The CatWISE Preliminary Catalog: motions from WISE and NEOWISE data.
o	<CWISEP JHHMMSS.ss+DDMMSS.s> N~1000000000. <CWISEPR JHHMMSS.ss+DDMMSS.s> N=111394986. JPL/Caltech
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CWISER
CWISER	(CatWISE Reject file) (Not yet in Simbad)
Write:	<<CWISER JHHMMSS.ss+DDMMSS.s>>
N:	111394986 (SIMBAD class: MidIR = Mid-IR Source (3 to 30 µm))
Note:	CatWISE is a full-sky catalog consisting of sources selected at 3.4 and 4.6 microns from four years of WISE and NEOWISE survey data. The Reject file consists of sources which do NOT satisfy the following criteria: 1) Primary in tile. As in WISE, the area of the sky is divided into 18,240 tiles which have some overlap and hence duplicate source entries. The primary in tile designation means the source is further from the tile edge than are the duplicate entries. 2) Have no identified artifact and SNR ≥ 5 at 3.4 microns, or have no identified artifact and SNR ≥ 5 at 4.6 microns.
Notes:	CatWISE data overview paper (to be submitted in March); Discovery of a very cool Y dwarf with CatWISE (to be submitted in March) See also CWISEPR for the preliminary release.
Ref:	=2021ApJS..253....8M
by	MAROCCO F. , EISENHARDT P.R.M., FOWLER J.W., KIRKPATRICK J.D., MEISNER A.M., SCHLAFLY E.F., STANFORD S.A., GARCIA N., CASELDEN D., CUSHING M.C., CUTRI R.M., FAHERTY J.K., GELINO C.R., GONZALEZ A.H., JARRETT T.H., KOONTZ R., MAINZER A., MARCHESE E.J., MOBASHER B., SCHLEGEL D.J., STERN D., TEPLITZ H.I., WRIGHT E.L.
	Astrophys. J., Suppl. Ser., 253, 8-8 (2021)
	The CatWISE2020 Catalog.
o	<CWISE JHHMMSS.ss+DDMMSS.s> N≃1000000000. <CWISER JHHMMSS.ss+DDMMSS.s> N=111394986. JPL/Caltech
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [CWL2004]
[CWL2004]	(Chandar+Whitmore +Lee, 2004) (Not yet in Simbad)
Write:	<<[CWL2004] M NNN NN>> <<[CWL2004] NGC 6946 NN>>
N:	47+21+19+29+34
Object:	Poss. GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	HST WFPC2 images of 5 galaxies to study ancient star cluster populations.
in source:	M 81 = NGC 3031
in source:	M 83 = NGC 5236
in source:	NGC 6946
in source:	M 101 = NGC 5457
in source:	M 51 = NGC 5194
Ref:	=2004ApJ...611..220C
by	CHANDAR R. , WHITMORE B., LEE M.G.
	Astrophys. J., 611, 220-244 (2004)
	The globular cluster systems of five nearby spiral galaxies: new insights from Hubble space telescope imaging.
o	Table 3: <[CWL2004] M 81 NN> (Nos 1-47). Table 4: <[CWL2004] M 83 NN> (Nos 1-21). Table 5: <[CWL2004] NGC 6946 NN> (Nos 1-19). Table 6: <[CWL2004] M 101 NN> (Nos 1-29). Table 7: <[CWL2004] M 51 NN> (Nos 1-34).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWM2017]
[CWM2017]	(Caldwell+Walker+Mateo+, 2017)
Write:	<<[CWM2017] Cra2-NNN>>
N:	404
Object:	Poss. RGB* (SIMBAD class: RGB*_Candidate = Red Giant Branch star Candidate)
Note:	MMT Hectochelle spectroscopic observations of N=404 red giant candidate stars in the field of Crater II dwarf galaxy. Use of the archival VST-ATLAS survey.
in source:	NAME Crater II
Ref:	=2017ApJ...839...20C
by	CALDWELL N. , WALKER M.G., MATEO M., OLSZEWSKI E.W., KOPOSOV S., BELOKUROV V., TORREALBA G., GERINGER-SAMETH A., JOHNSON C.I.
	Astrophys. J., 839, 20-20 (2017)
	Crater 2: an extremely cold dark matter halo.
o	(Erratum) erratum vol. 841, art. 66 (2017)
o	Table 2: <[CWM2017] Cra2-NNN> (Nos 1-404).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWN2006]
[CWN2006]	(Cartwright+Whitworth+Nutter, 2006) (Not yet in Simbad)
Write:	<<[CWN2006] Ori B Cluster N>>
N:	3
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Three distinct star clusters or cores are seen by SCUBA at the JCMT in Ori B.
in source:	NAME Ori B
Ref:	=2006MNRAS.369.1411C
by	CARTWRIGHT A. , WHITWORTH A.P., NUTTER D.
	Mon. Not. R. Astron. Soc., 369, 1411-1418 (2006)
	Methods for analysing structure in molecular clouds.
o	Fig.2: <[CWN2006] Ori B CLuster N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWO2003]
[CWO2003]	(Chapman+Windhorst+Odewahn+, 2003)= (SMM)
Write:	<<[CWO2003] SMM JHHMMSS.s+DDMMSS>>
N:	13
Object:	(Sub-mm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	HST STIS imaging of 13 submillimeter luminous galaxies.
Ref:	=2003ApJ...599...92C
by	CHAPMAN S.C. , WINDHORST R., ODEWAHN S., YAN H., CONSELICE C.
	Astrophys. J., 599, 92-104 (2003)
	Hubble Space Telescope images of submillimeter sources: large irregular galaxies at high redshift.
o	Table 1, Fig.2: <[CWO2003] SMM JHHMMSS.s+DDMMSS> N=13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWO2004]
[CWO2004]	(Crighton+Webb+Ortiz-Gil+, 2004)
Write:	<<[CWO2004] QSO J1939-1002 abs N.NNN>>
N:	1
Object:	DLA
Note:	New DLA system at z = 3.256 towards PKS 1937-101 = QSO J1939-1002.
Ref:	=2004MNRAS.355.1042C
by	CRIGHTON N.H.M. , WEBB J.K., ORTIZ-GIL A., FERNANDEZ-SOTO A.
	Mon. Not. R. Astron. Soc., 355, 1042-1052 (2004)
	Deuterium/hydrogen in a new Lyman limit absorption system at z= 3.256 towards PKS1937-1009.
o	PKS1937-1009 = PKS 1937-101 and PG 1718-4801 = PG 1718-481 in SIMBAD.
o	Text: <[CWO2004] QSO J1939-1002 abs N.NNN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWP2005]
[CWP2005]	(Cooke+Wolfe+Prochaska+, 2005)
Write:	<<[CWP2005] QSO JHHMM+DDMM abs N.NNN>>
N:	2
Object:	DLA
Note:	Imaging at the Palomar and Keck Observatories. Among the DLAs in QSOs spectra at z about 3, 2 were not yet identified in the spectra of PSS J0808+5215 = QSO J0808+5215, and OC 1643+4631A = QSO J1645+4626.
Ref:	=2005ApJ...621..596C
by	COOKE J. , WOLFE A.M., PROCHASKA J.X., GAWISER E.
	Astrophys. J., 621, 596-614 (2005)
	Survey for galaxies associated with z ~ 3 damped Lyα systems. I. Spectroscopic calibration of u'BVRI photometric selection.
o	Table 1: DLAs which are not '[CWP2005]' objects are already known with an other ID.
o	Table 1: <[CWP2005] QSO JHHMM+DDMM abs N.NNN> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWP2007]
[CWP2007]	(Churchwell+Watson+Povich+, 2007)
Write:	<<[CWP2007] CW NNN>>
N:	151+118
Object:	Bubble (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Spitzer GLIMPSE II legacy science program images.
Ref:	=2007ApJ...670..428C
by	CHURCHWELL E. , WATSON D.F., POVICH M.S., TAYLOR M.G., BABLER B.L., MEADE M.R., BENJAMIN R.A., INDEBETOUW R., WHITNEY B.A.
	Astrophys. J., 670, 428-441 (2007)
	The bubbling galactic disk. II. The inner 20°.
o	Table 1: <[CWP2007] CN NNN> (Nos 1-151). Table 2: <[CWP2007] CS NNN> (Nos 1-118).
=E=	Catalogue in electronic form as J/ApJ/670/428
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWP2012]
[CWP2012]	(CHEN+WILLIAMS+PANDIAN, 2012)
Write:	<<[CWP2012] Sh2-157B-MMN>> <<[CWP2012] Sh2-157B-IRN>>
N:	8
Object:	(mm) + (IR) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	SMA 220 GHz continuum and Infrared Telescope Facility MIRSI observations of Sh 2-157.
in source:	SH 2-157
Ref:	=2012ApJ...752..102C
by	CHEN C.-C. , WILLIAMS J.P., PANDIAN J.D.
	Astrophys. J., 752, 102 (2012)
	H II regions, embedded protostars, and starless cores in Sharpless 2-157.
o	Table 2: <[CWP2012] Sh2-157B-MMN> (Nos MM1-MM6), Table 3: <[CWP2012] Sh2-157B-IRN> (Nos IRS1-IRS2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWP2012b]
[CWP2012b]	(Capelli+Warwick+Porquet+, 2012)
Write:	<<[CWP2012b] AN>> <<[CWP2012b] DSN>> <<[CWP2012b] EDE>> <<[CWP2012b] EDW>>
N:	14 (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton EPICMOS observations targeted at Sgr A*.
in source:	NAME Gal Center
Ref:	=2012A&A...545A..35C
by	CAPELLI R. , WARWICK R.S., PORQUET D., GILLESSEN S., PREDEHL P.
	Astron. Astrophys., 545A, 35-35 (2012)
	The X-ray lightcurve of Sagittarius A over the past 150 years inferred* from Fe-Kα line reverberation in Galactic centre molecular clouds.
o	Table 2 <[CWP2012b] AN>(Nos A, B1-B2, C-F, F1-F3), <[CWP2012b] DSN>(Nos DS1-DS2), <[CWP2012b] EDE>(Nos EDE, EDW), N=14
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWP97]
[CWP97]	(Clocchiatti+Wheeler+Phillips+, 1997) (Not yet in Simbad)
Write:	<<[CWP97] N>>
N:	4
Object:	* (SIMBAD class: Star)
Note:	Stars around NGC 1365.
Ref:	=1997ApJ...483..675C
by	CLOCCHIATTI A. , WHEELER J.C., PHILLIPS M.M., SUNTZEFF N.B., CRISTIANI S., PHILLIPS A., HARKNESS R.P., DOPITA M.A., BEUERMANN K., ROSA M., GROSBOL P., LINDBLAD P.O., FILIPPENKO A.V.
	Astrophys. J., 483, 675-697 (1997)
	SN 1983V in NGC 1365 and the nature of stripped envelope core-collapse supernovae.
o	Table 2: stars are not in SIMBAD
o	Table 2: <[CWP97] N> (Nos 1-4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CWRU
CWRU	(Case Western Reserve Univ.) (Not yet in Simbad)
Write:	<<CWRU N>>
N:	1
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Details on Acronym: [CWS2005]
[CWS2005]	(Cannon+Walter+Skillman+, 2005)= ([CWS2005a])
Write:	<<[CWS2005] I Zw 18 WW>> <<[CWS2005] I Zw 18 WW-A>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA observations of Zw I 18: N=4 radio continuum emission sources. Use of HST archival data. See also [DKF89], [CSG2002].
in source:	Zw I 18 = Mrk 116
Ref:	=2005ApJ...621L..21C
by	CANNON J.M. , WALTER F., SKILLMAN E.D., VAN ZEE L.
	Astrophys. J., 621, 21-24 (2005)
	The nature of radio continuum emission at very low metallicity: Very Large Array observations of I Zw 18.
o	Table 1: <[CWS2005] I Zw 18 WW> (No. SE), <[CWS2005] I Zw 18 WW-A> (Nos NW-A to NW-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWS2005a]
[CWS2005a]	(Cannon+Walter+Skillman+, 2005)
*****	Avoid the usage of [CWS2005a], prefer [CWS2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWS2005b]
[CWS2005b]	(Carpano+Wilms+Schirmer+, 2005)
Write:	<<[CWS2005b] NNN>>
N:	163
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Optical identification with observations from the 2.2 MPG-ESO telescope in La Silla of NGC 300.
in source:	NGC 300
Ref:	=2005A&A...443..103C
by	CARPANO S. , WILMS J., SCHIRMER M., KENDZIORRA E.
	Astron. Astrophys., 443, 103-114 (2005)
	X-ray properties of NGC 300. I. Global properties of X-ray point sources and their optical counterparts.
o	Table 1: <[CWS2005b] NNN> (Nos 1-163).
=E=	Catalogue in electronic form as J/A+A/443/103
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWS2017]
[CWS2017]	(Cole+Weisz+Skillman+, 2017)
Write:	<<[CWS2017] NNNNN>>
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	HST ACS observations of N=36 variable stars in the central cluster [HM82] A1 of the Pegasus dwarf irregular galaxy.
in source:	NAME Peg Dwarf Irregular Galaxy: [HM82] A1 = [HM82] A1
Ref:	=2017ApJ...837...54C
by	COLE A.A. , WEISZ D.R., SKILLMAN E.D., LEAMAN R., WILLIAMS B.F., DOLPHIN A.E., JOHNSON L.C., McCONNACHIE A.W., BOYLAN-KOLCHIN M., DALCANTON J., GOVERNATO F., MADAU P., SHEN S., VOGELSBERGER M.
	Astrophys. J., 837, 54-54 (2017)
	DDO 216-A1: a central globular cluster in a low-luminosity transition-type galaxy.
o	Table 1: <[CWS2017] NNNNN> N=36 among (Nos 16415-40802).
=E=	Catalogue in electronic form as <J/ApJ/837/54/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWT2009]
[CWT2009]	(Crivellari+Wolter+Trinchieri, 2009)
Write:	<<[CWT2009] XMM NN>>
N:	11
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton EPIC observations of the Cartwheel galaxy.
in source:	NAME Cartwheel Galaxy
Ref:	=2009A&A...501..445C
by	CRIVELLARI E. , WOLTER A., TRINCHIERI G.
	Astron. Astrophys., 501, 445-453 (2009)
	The Cartwheel galaxy with XMM-Newton.
o	Table 2: <[CWT2009] XMM NN> (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CWW
CWW	(Curtis+Wolfgang+Wright)
*****	Avoid the usage of CWW, prefer [CWW2013]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CWW2011]
[CWW2011]	(Curran+Whitting+Webb+, 2011) (Not yet in Simbad)
Write:	<<[CWW2011] A>>
N:	4
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Host galaxy (H) and three absorption features (A, B, C) within the SW lobe of PKS 1649-062.
Ref:	=2011MNRAS.414L..26C
by	CURRAN S.J. , WHITING M.T., WEBB J.K., ATHREYA R.
	Mon. Not. R. Astron. Soc., 414L, 26-30 (2011)
	Localized H I 21-cm absorption towards a double-lobed z= 0.24 radio galaxy.
o	Fig. 5, Table 2: <[CWW2011] A> (Nos A-C, H).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CWW2013]
[CWW2013]	(Curtis+Wolfgang+Wright+, 2013)= (CWW)
Write:	<<[CWW2013] NNN>>
N:	108
Object:	* (SIMBAD class: Star)
Note:	Lick Shane telescope, Palomar Hale telescope and MMT Hectochelle radial velocities measurements and CFHT MegaCam (g'r'i'z') photometry of N=108 stars in Ruprecht 147.
in source:	Cl Ruprecht 147
Ref:	=2013AJ....145..134C
by	CURTIS J.L. , WOLFGANG A., WRIGHT J.T., BREWER J.M., JOHNSON J.A.
	Astron. J., 145, 134 (2013)
	Ruprecht 147: the oldest nearby open cluster as a new benchmark for stellar astrophysics.
o	Table 3: <[CWW2013] NNN> (Nos 1-108).
=E=	Catalogue in electronic form as <J/AJ/145/134/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CX
CX	(Chandra X-ray)
*****	Avoid the usage of CX, prefer [BPH2004]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CX
CX	(Chandra X-ray)
*****	Avoid the usage of CX, prefer [CWH2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CX
CX	(Chandra X-ray)
*****	Avoid the usage of CX, prefer CXO
Origin	of the Acronym: L (2000ApJ...531L...9K)
Details on Acronym: CX
CX	(Chandra X-ray)
*****	Avoid the usage of CX, prefer [HWC2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CX
CX	(Chandra, X-ray)
*****	Avoid the usage of CX, prefer [VTB2004]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CXCAnt
CXCAnt	(Chandra X-ray Catalog , Antennae)
Write:	<<CXCAnt JHHMMSS.s+DDMMSS>>
N:	120
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS-S multi-epoch observations of The Antennae. See also [ZFB2006] and CXOAnt.
in source:	NAME the Antennae
Ref:	=2006ApJS..166..211Z
by	ZEZAS A. , FABBIANO G., BALDI A., SCHWEIZER F., KING A.R., PONMAN T.J., ROTS A.H.
	Astrophys. J., Suppl. Ser., 166, 211-248 (2006)
	Chandra monitoring observations of The Antennae galaxies. I. Catalog of source properties.
o	Table 3: <[ZFB2006] NNN> (Nos 1-120) = Table 5: <CXCAnt JHHMMSS.s+DDMMSS> N=120. End of Table 5: <[ZFB2006] N D> (Nos 1 D to 7 D).
=E=	Catalogue in electronic form as J/ApJS/166/211
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CXCCLASXS
CXCCLASXS	(Chandra X-ray Catalog from the CLASXS)
Write:	<<CXCCLASXS JHHMMSS.s+DDMMSS>>
N:	525
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	X-ray catalog from the Chandra Large Area Synoptic X-ray Survey (CLASXS). A second designation with a runing number is also used by the authors, see CLASXS.
in source:	NAME Lockman Hole Northwest Field
Ref:	=2004AJ....128.1501Y
by	YANG Y. , MUSHOTZKY R.F., STEFFEN A.T., BARGER A.J., COWIE L.L.
	Astron. J., 128, 1501-1523 (2004)
	The Chandra large area synoptic X-ray survey (CLASXS) of the Lockman Hole-northwest: the X-ray catalog.
o	Table 2, col(1): <CLASXS NNN> (Nos 1-525) = Table 2, col(2): <CXCCLASXS JHHMMSS.s+DDMMSS> N=525. Table 4: <[YMS2004] N> (Nos 1-4).
=E=	Catalogue in electronic form as J/AJ/128/1501
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CXD2016]
[CXD2016]	(Cao+Xu+Domingue+, 2016) (Not yet in Simbad)
Write:	<<[CXD2016] btsh-NNN>> <<[CXD2016] egs-NNN>> <<[CXD2016] en1-NNN>> <<[CXD2016] lk-NNN>>
N:	132
Object:	G (SIMBAD class: Galaxy)
Note:	N=172 galaxies, part of a control sample selected from 2MASS galaxies with Herschel data, as part of a study of close major-merger pairs of galaxies. See also KPAIR and [XDC010].
Ref:	=2016ApJS..222...16C
by	CAO C. , XU C.K., DOMINGUE D., BUAT V., CHENG Y.-W., GAO Y., HUANG J., JARRETT T.H., LISENFELD U., LU N., MAZZARELLA J., SUN W.-H., WU H., YUN M.S., RONCA J., JACQUES A.
	Astrophys. J., Suppl. Ser., 222, 16 (2016)
	Herschel observations of Major merger pairs at z = 0: dust mass and star formation.
o	Table 1: <KPAIR JHHMM+DDMM> N=66 added. Table 4: <[CXD2016] btsh-NNN> N=14 among (Nos 004-212), <[CXD2016] egs-NNN> N=12 among (Nos 005-066), <[CXD2016] en1-NNN> N=9 among (Nos 003-048), <[CXD2016] lk-NNN> N=97 among (Nos 006-416).
=E=	Catalogue in electronic form as <J/ApJS/222/16/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CXGCS
CXGCS	(Chandra X-ray, Galactic Center Survey)
*****	Avoid the usage of CXGCS, prefer CXOGCS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CXH
CXH	(Cygnus X, Hole)
Write:	<<CXH N>>
N:	6
Object:	Hole (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Table 7: (Nos 1-6), Holes in Cygnus X
in source:	NAME Cyg X
Ref:	=1991A&A...241..551W
by	WENDKER H.J. , HIGGS L.A., LANDECKER T.L.
	Astron. Astrophys., 241, 551-580 (1991)
	The Cygnus X region. XVIII. A detailed investigation of radio-continuum structure on large and small scales.
o	Table 2: <18P NNNA> (Nos 1-103), N=109. Table 3: <19P NNA> (Nos 1-48), N=50. Table 4: <EXC6-NNA> (Nos 1-41), N=47. Table 6: <CXR NN> (Nos 1-13), N=13, Table 7: <CXH N> (Nos 1-6), N=6
=E=	Catalogue in electronic form as J/A+A/241/551
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CXL2021]
[CXL2021]	(Cui+Xin+Liu+, 2021)
Write:	<<[CXL2021] SrcXN>>
N:	2
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	N=2 GeV sources, discovered in Fermi LAT data, in the vicinity of HESS J1858+020.
Ref:	=2021A&A...646A.114C
by	CUI Y. , XIN Y., LIU S., TAM P.H.T., PUHLHOFER G., ZHU H.
	Astron. Astrophys., 646A, 114-114 (2021)
	HESS J1858+020: A GeV-TeV source possibly powered by cosmic rays from SNR G35.6-0.4.
o	Fig. 1, Table 1: <[CXL2021] SrcXN> (Nos SrcX1-SrcX2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CXO
CXO	(Chandra X-ray Observatory)= (CX)
Write:	<<CXO JHHMMSS.s+DDMMSS>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Standard designation for sources detected in observations made with the Chandra X-ray Observatory. There are 3 standard designations for sources detected in observations made with the Chandra X-ray Observatory. CXO is reserved for use by the Chandra X-ray Observatory Center (CXC) for designating sources from projects of an institutional nature. CXOAA, CXOAAA, and CXOAAAA (i.e., "CXO" with two, three, or four appended characters) are available for comprehensive source lists derived from Chandra observations and made by individuals who pre-register the acronym using the IAU form at http://cdsweb.u-strasbg.fr/viz-bin/DicForm where they indicate the meaning of the appended characters, which are usually the initials of the author(s). CXOU where U means "unregistered" may be used for the occasional sources found/published by individuals using Chandra X-ray Observatory data. The Chandra Source Catalog is described in Evans et al. (2010ApJS..189...37E), and available at: http://cxc.cfa.harvard.edu/csc/
Ref:	=2010ApJS..189...37E
by	EVANS I.N. , PRIMINI F.A., GLOTFELTY K.J., ANDERSON C.S., BONAVENTURA N.R., CHEN J.C., DAVIS J.E., DOE S.M., EVANS J.D., FABBIANO G., GALLE E.C., GIBBS D.G., GRIER J.D., HAIN R.M., HALL D.M., HARBO P.N., HE X., HOUCK J.C., KAROVSKA M., KASHYAP V.L., LAUER J., McCOLLOUGH M.L., McDOWELL J.C., MILLER J.B., MITSCHANG A.W., MORGAN D.L., MOSSMAN A.E., NICHOLS J.S., NOWAK M.A., PLUMMER D.A., REFSDAL B.L., ROTS A.H., SIEMIGINOWSKA A., SUNDHEIM B.A., TIBBETTS M.S., VAN STONE D.W., WINKELMAN S.L., ZOGRAFOU P.
	Astrophys. J., Suppl. Ser., 189, 37-82 (2010)
	The Chandra source catalog.
o	<CXO JHHMMSS.s+DDMMSS> N=94676. CfA / Chandra X-ray observatory Center
=E=	Catalogue in electronic form as <IX/45/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXO
CXO	(Simon, 2009)
*****	Avoid the usage of CXO, prefer [S2009b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 2CXO
2CXO	(Second release of the Chandra Source Catalog)
Write:	<<2CXO JHHMMSS.s+DDMMSS{\|X}>>
N:	about 150000
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	The second release of the Chandra Source Catalog (CSC) is currently under development and is expected early 2014, but we would like to pre-register the acronym. Its nature is identical to the CXO acronym which we reserved exclusively for the first release of the CSC, with one exception: while the first release contained only compact (i.e., unresolved) sources, in this release we will include extended sources as well; if there would a be naming conflict between a compact and an extended source, we will append the letter 'X' to the source name to identify the extended source. Consequently, a source whose name ends in 'X' will be guaranteed to be extended; all other sources may be compact or extended. The rationale for not explicitly identifying compact sources is the large variation in PSF size over Chandra's field of view which makes a specific compact designation meaningless.
Auth.:	Arnold Rots Smithsonian Astrophysical Observatory
=E=	Catalogue in electronic form as <IX/57/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOANC
CXOANC	(Chandra X-ray Observatory, ANCHORS)
Write:	<<CXOANC JHHMMSS.s+DDMMSS>>
N:	about 4000
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	In preparation. Database of all X-ray sources in regions of star formation. The data include: source positions, count rates, spectral fits, X-ray colors, 2MASS, IRAS and optical matches. The prototype web site is at: http://hea-www.harvard.edu/~swolk/ANCHORS/.br a working page is at http://hea-www.harvard.edu/~swolk/ANCHORS/00642/obs.htmlbr 2007AJ....134..411M: first ref. with N=11 CXOANC objects.
Auth.:	WOLK S.
Ref:	=2007AJ....134..411M
by	MUENCH A.A. , LADA C.J., LUHMAN K.L., MUZEROLLE J., YOUNG E.
	Astron. J., 134, 411-444 (2007)
	A Spitzer census of the IC 348 nebula.
o	Cl* IC 348 LRL 10019 = Cl* IC 348 CB 136 not Cl* IC 348 CB 138; Cl* IC 348 LRL 10138 = Cl* IC 348 CB 139 not Cl* IC 348 CB 141; Cl* IC 348 LRL 54916 = Cl* IC 348 CB 114 not Cl* IC 348 CB 116
o	Tables 1-2, 7, 11: <Cl* IC 348 LRL NNNNN> N=368 among (Nos 1-57025). Table 4: <[MLL2007] MMS N> (Nos 1-7), <[MLL2007] MMP NN> (Nos 1-19). Table 11: <CXOANC JHHMMSS.s+DDMMSS> N=10.
=E=	Catalogue in electronic form as J/AJ/134/411
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOAnt
CXOAnt	(Chandra, Antennae)
Write:	<<CXOAnt JHHMMSS.s+DDMMSS.s>>
N:	53
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Study of the Antennae galaxies (NGC4038/39) in the X-rays with the Chandra X-ray Observatory. See also [ZFR2002], CXCAnt, [ZFB2006].
in source:	NAME the Antennae
Ref:	=2002ApJS..142..239Z
by	ZEZAS A. , FABBIANO G., ROTS A.H., MURRAY S.S.
	Astrophys. J., Suppl. Ser., 142, 239-260 (2002)
	Chandra observations of "The Antennae" galaxies (NGC 4038/4039). II. Detection and analysis of galaxian X-ray sources.
o	Table 1, col(1): <[ZFR2002] NN> (Nos 1-49), <[ZFR2002] Nc> (Nos 1c-3c) = Table 1, col(2): <CXOAnt JHHMMSS.s+DDMMSS.s> N=52.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOAYSB
CXOAYSB	(Chandra, Aybuke Kupcu-Yoldas+Solen Balman)
Write:	<<CXOAYSB JHHMMSS.s+DDMMSS.s>>
N:	16
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Detection of 16 new X-ray sources with CHANDRA ACIS DETECTOR. The sources are detected in a pointed obseravtion of the Classical Nova shell of GK Persei (a cataclysmic variable). The observation was a 100ksec deep exposure with ACIS-S (grating NONE). The 16 sources that are detected all have low X-ray flux ( 10^–14 erg/cm²/s) which are at least 5-6 sigma above the background. They are not listed in any other catalogue and are unknown in nature. Some object names are built from truncated coordinates, and others from rounded coordinates.
Ref:	=2002A&A...384..190K
by	KUEPCUE YOLDAS A. , BALMAN S.
	Astron. Astrophys., 384, 190-194 (2002)
	CHANDRA detection of 16 new X-ray sources.
o	Table 1: <CXOAYSB JHHMMSS.s+DDMMSS.s> N=16.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOC
CXOC	(Chandra X-ray Observatory COSMOS survey)
Write:	<<CXOC JHHMMSS.s+DDMMSS>>
N:	1761
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	The Chandra COSMOS Survey (C-COSMOS) of the central 0.5 square degrees of the COSMOS field. See also [ECV2009].
in source:	NAME COSMOS Field
Ref:	=2009ApJS..184..158E
by	ELVIS M. , CIVANO F., VIGNALI C., PUCCETTI S., FIORE F., CAPPELLUTI N., ALDCROFT T.L., FRUSCIONE A., ZAMORANI G., COMASTRI A., BRUSA M., GILLI R., MIYAJI T., DAMIANI F., KOEKEMOER A.M., FINOGUENOV A., BRUNNER H., URRY C.M., SILVERMAN J., MAINIERI V., HASINGER G., GRIFFITHS R., CAROLLO M., HAO H., GUZZO L., BLAIN A., CALZETTI D., CARILLI C., CAPAK P., ETTORI S., FABBIANO G., IMPEY C., LILLY S., MOBASHER B., RICH M., SALVATO M., SANDERS D.B., SCHINNERER E., SCOVILLE N., SHOPBELL P., TAYLOR J.E., TANIGUCHI Y., VOLONTERI M.
	Astrophys. J., Suppl. Ser., 184, 158-171 (2009)
	The Chandra COSMOS survey. I. Overview and point source catalog.
o	Catalog, col(1): <CXOC JHHMMSS.s+DDMMSS> N=1761 = Catalog, col(2): <[ECV2009] NNNNN> N=1761 among (Nos 1-22962).
=E=	Catalogue in electronic form as J/ApJS/184/158
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CXOCDFS
CXOCDFS	(Chandra, Deep Field South)
Write:	<<CXOCDFS JHHMMSS.s+DDMMSS>>
N:	346
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	The Chandra Deep Field South currently consists of a combined 940 ksec exposure using ACIS-I on-board the Chandra X-ray Observatory. The pointing covers 0.096 square degrees and has resulted in a catalog of roughly 300 sources with S/N greater than 2. See also [GZW2002].
in source:	NAME CDFS
Ref:	=2002ApJS..139..369G
by	GIACCONI R. , ZIRM A., WANG J., ROSATI P., NONINO M., TOZZI P., GILLI R., MAINIERI V., HASINGER G., KEWLEY L., BERGERON J., BORGANI S., GILMOZZI R., GROGIN N., KOEKEMOER A., SCHREIER E., ZHENG W., NORMAN C.
	Astrophys. J., Suppl. Ser., 139, 369-410 (2002)
	Chandra Deep Field South: the 1 Ms catalog.
o	CXOCDFS J033260.0-274748 translated into CXOCDFS J033300.0-274748
o	Table 2: <[GZW2002] Main NNN> (Nos 1-304) = <[GZW2002] XID NNN> N=304 = <CXOCDFS JHHMMSS.s+DDMMSS> N=304. Table 3: <[GZW2002] SExtractor NN> (Nos 1-28) = <[GZW2002] XID NNN> N=28 = <CXOCDFS JHHMMSS.s+DDMMSS> N=28. Table 4: <[GZW2002] WAVDETECT NN> (Nos 1-14) = <[GZW2002] XID NNN> N=14 = <CXOCDFS JHHMMSS.s+DDMMSS> N=14.
=E=	Catalogue in electronic form as J/ApJS/139/369
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOCepB
CXOCepB	(Chandra X-ray Observatory, Cep B)
Write:	<<CXOCepB JHHMMSS.ss+DDMMSS.s>>
N:	431
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra study of the Cep B molecular cloud. See also [GFT2006].
Ref:	=2006ApJS..163..306G
by	GETMAN K.V. , FEIGELSON E.D., TOWNSLEY L., BROOS P., GARMIRE G., TSUJIMOTO M.
	Astrophys. J., Suppl. Ser., 163, 306-334 (2006)
	Chandra study of the Cepheus B star-forming region: stellar populations and the initial mass function.
o	Table 1, col(1): <[GFT2006] NNN> (Nos 1-431) = Table 1, col(2): <CXOCepB JHHMMSS.ss+DDMMSS.s> N=431.
=E=	Catalogue in electronic form as J/ApJS/163/306
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CXOCOB2
CXOCOB2	(Chandra X-ray Observatory, Cyg OB2)
Write:	<<CXOCOB2 JHHMMSS.ss+DDMMSS.s>>
N:	7924
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Catalogue of N=7924 X-ray sources, as part of the Chandra Cygnus OB2 Legacy Survey. See also [WDG2023].
in source:	NAME VI CYG = Ass Cyg OB 2
Ref:	=2023ApJS..269....7W
by	WRIGHT N.J. , DRAKE J.J., GUARCELLO M.G., ALDCROFT T.L., KASHYAP V.L., DAMIANI F., DEPASQUALE J., FRUSCIONE A.
	Astrophys. J., Suppl. Ser., 269, 7 (2023)
	The Chandra Cygnus OB2 Legacy Survey: Design and X-Ray Point-source Catalog.
o	Table 2, col(1): <[WDG2023] NNNN> (Nos 1-7924) = Table 2, col(2): <CXOCOB2 JHHMSS.ss+DDMMSS.s> N=7924.
=E=	Catalogue in electronic form as <J/ApJS/269/7/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CXOComa
CXOComa	(Chandra X-ray Observatory, Coma cluster)
Write:	<<CXOComa JHHMMSS.ss+DDMMSS.s>>
N:	13+3
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra study of a Coma Cluster off-center region. T.2: 3 sources are undetected. See also [MBC2001].
in source:	Coma Cluster = ACO 1656
Ref:	=2006ApJ...643..144H
by	HORNSCHEMEIER A.E. , MOBASHER B., ALEXANDER D.M., BAUER F.E., BAUTZ M.W., HAMMER D., POGGIANTI B.M.
	Astrophys. J., 643, 144-153 (2006)
	Chandra X-ray observations of galaxies in an off-center region of the Coma cluster.
o	Paragr.4: CXOComa J123815.1+272927 is a misprint for CXOComa J125815.13+272927.1
o	Tables 1, 2: <CXOComa JHHMMSS.ss+DDMMSS.s> N=13+3.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CXOCY
CXOCY	(Chandra X-ray Observatory, Calan Yale)
Write:	<<CXOCY JHHMMSS.s+DDMMSS>>
N:	267
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	The CYDER (Calan Yale Deep Extragalactic Research) survey is a survey to study faint extragalactic populations. Part of the survey is carried out in archival Chandra deep fields to study the X-ray sources optical counterparts. We are thus identifying Chandra X-ray sources that we would like to name with the proposed acronym. 2003AJ....125.1689C: first ref. with a CXOCY object.
in source:	NAME CDFN
in source:	NAME CDFS
Ref:	=2003AJ....125.1689C
by	CASTANDER F.J. , TREISTER E., MACCARONE T.J., COPPI P.S., MAZA J., ZEPF S.E., GUZMAN R.
	Astron. J., 125, 1689-1695 (2003)
	High-redshift X-Ray-Selected quasars: CXOCY J125304.0-090737 joins the club.
o	<CXOCY JHHMMSS.s+DDMMSS> N=1.
Ref:	=2005ApJ...621..104T
by	TREISTER E. , CASTANDER F.J., MACCARONE T.J., GAWISER E., COPPI P.S., URRY C.M., MAZA J., HERRERA D., GONZALEZ V., MONTOYA C., PINEDA P.
	Astrophys. J., 621, 104-122 (2005)
	The Calan-Yale Deep Extragalactic Research (CYDER) survey: optical properties and deep spectroscopy of serendipitous X-ray sources.
o	Table 4: <CXOCY JHHMMSS.s+DDMMSS> N=267.
=E=	Catalogue in electronic form as J/ApJ/621/104
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOCyg
CXOCyg	(Chandra X-ray Observatory, Cyg OB2)
Write:	<<CXOCyg JHHMMSS.ss+DDMMSS.s>>
N:	1003
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	X-ray source detection and analysis in the Cygnus OB2 region. See also [AFM2007].
in source:	Ass Cyg OB 2 = NAME VI CYG
Ref:	=2007A&A...464..211A
by	ALBACETE COLOMBO J.F. , FLACCOMIO E., MICELA G., SCIORTINO S., DAMIANI F.
	Astron. Astrophys., 464, 211-227 (2007)
	Unveiling the Cygnus OB2 stellar population with Chandra.
o	Table 1, col(1): <[AFM2007] NNNN> (Nos 1-1003) = Table 1, col(2): <CXOCyg JHHMMSS.ss+DDMMSS.s> N=1003.
=E=	Catalogue in electronic form as J/A+A/464/211
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOECDFS
CXOECDFS	(Chandra X-ray Observatory, Extended, CDFS)
Write:	<<CXOECDFS JHHMMSS.s-DDMMSS>>
N:	762+33
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Extended-Chandra Deep-Field South catalog. The E-CDF-S is comprised of four deep (250 ks) Chandra fields flanking the original 1 Ms CDFS. These cover about 0.3 square degrees, about 3.5 times the solid angle of the original CDFS. See also [LBA2005].
Ref:	=2005ApJS..161...21L
by	LEHMER B.D. , BRANDT W.N., ALEXANDER D.M., BAUER F.E., SCHNEIDER D.P., TOZZI P., BERGERON J., GARMIRE G.P., GIACCONI R., GILLI R., HASINGER G., HORNSCHEMEIER A.E., KOEKEMOER A.M., MAINIERI V., MIYAJI T., NONINO M., ROSATI P., SILVERMAN J.D., SZOKOLY G., VIGNALI C.
	Astrophys. J., Suppl. Ser., 161, 21-40 (2005)
	The Extended Chandra Deep Field-South survey: Chandra point-source catalogs.
o	Tables 2, 6, col(1): <[LBA2005] NNN> (Nos 1-762) = <CXOECDFS JHHMMSS.s-DDMMSS> N=762, <[LBA2005] SNN> (Nos S1-S33) = <CXOECDFS JHHMMSS.s-DDMMSS> N=33.
=E=	Catalogue in electronic form as J/ApJS/161/21
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOEGS
CXOEGS	(Chandra X-ray Observatory, Extended Groth Strip)
Write:	<<CXOEGS JHHMMSS.s+DDMMSS>>
N:	1325
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Catalog which refers to X-ray sources in the Chandra survey of the Extended Groth Strip: CXOGWS (Groth-Westphal Strip) has now been extended to the region known as the Extended Groth Strip. See also [LNG2009].
in source:	NAME Extended Groth Strip
Ref:	=2009ApJS..180..102L
by	LAIRD E.S. , NANDRA K., GEORGAKAKIS A., AIRD J.A., BARMBY P., CONSELICE C.J., COIL A.L., DAVIS M., FABER S.M., FAZIO G.G., GUHATHAKURTA P., KOO D.C., SARAJEDINI V., WILLMER C.N.A.
	Astrophys. J., Suppl. Ser., 180, 102-116 (2009)
	AEGIS-X: the Chandra Deep Survey of the Extended Groth Strip.
o	Table 9, col(1): <[LNG2009] egs-NNNN> (Nos 1 to 1325) = Table 9, col(3): <CXOEGS JHHMMSS.s+DDMMSS> N=1325.
=E=	Catalogue in electronic form as J/ApJS/180/102
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOEN1
CXOEN1	(Chandra X-ray Observatory, ELAIS field N1)
Write:	<<CXOEN1 JHHMMSS.s+DDMMSS>>
N:	149+21
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	The ELAIS Deep X-ray Survey is being conducted in the European Large Area ISO survey field N1. See also CXOEN2, [MJA2003], [NLA2005]. We have 75 ks Chandra pointings in each field and a wealth of multiwavelength data including ISO 7.5, 15, 90, 175 um, SCUBA 850 um, VLA 1.4 GHz, g', r', i', H and K. XMM observations are awaiting scheduling.
in source:	ELAIS N1
Ref:	=2003MNRAS.343..293M
by	MANNERS J.C. , JOHNSON O., ALMAINI O., WILLOTT C.J., GONZALEZ-SOLARES E., LAWRENCE A., MANN R.G., PEREZ-FOURNON I., DUNLOP J.S., McMAHON R.G., OLIVER S.J., ROWAN-ROBINSON M., SERJEANT S.
	Mon. Not. R. Astron. Soc., 343, 293-305 (2003)
	The ELAIS deep X-ray survey - I. Chandra source catalogue and first results.
o	Table 1: <[MJA2003] N1-NNN> N=130 among (Nos N1-1 to N1-149) = <CXOEN1 JHHMMSS.s+DDMMSS> N=130. Table 2: <[MJA2003] N2-NNN> N=103 among (Nos N2-1 to N2-114) = <CXOEN2 JHHMMSS.s+DDMMSS> N=103.
Ref:	=2005MNRAS.356..568N
by	NANDRA K. , LAIRD E.S., ADELBERGER K., GARDNER J.P., MUSHOTZKY R.F., RHODES J., STEIDEL C.C., TEPLITZ H.I., ARNAUD K.A.
	Mon. Not. R. Astron. Soc., 356, 568-586 (2005)
	A deep Chandra survey of the Groth Strip - I. The X-ray data.
o	Table 3, col(1): <[NLA2005] cNNNN> (Nos c1-c158) = Table 3, col(2): <CXOGWS JHHMMSS.s+DDMMSS> N=158. Table A1, col(1): <[NLA2005] aNNN> N=21 among (Nos a6-a142) = Table A1, col(2): <CXOEN1 JHHMMSS.s+DDMMSS> N=21 added. Table A2, col(1): <[NLA2005] fNNN> N=75 among (Nos f9-f536) = Table A2, col(2): <CXOHDFN JHHMMSS.s+DDMMSS> N=75 added.
=E=	Catalogue in electronic form as J/MNRAS/343/293
=E=	Catalogue in electronic form as J/MNRAS/356/568
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOEN2
CXOEN2	(Chandra X-ray Observatory, ELAIS field N2)
Write:	<<CXOEN2 JHHMMSS.s+DDMMSS>>
N:	114
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	The ELAIS Deep X-ray Survey is being conducted in the European Large Area ISO survey field N2. See also CXOEN1, [MJA2003]. We have 75 ks Chandra pointings in each field and a wealth of multiwavelength data including ISO 7.5, 15, 90, 175 um, SCUBA 850 um, VLA 1.4 GHz, g', r', i', H and K. XMM observations are awaiting scheduling. 2003MNRAS.339..397W: first ref. with CXOEN2 objects.
in source:	ELAIS N2
Ref:	=2003MNRAS.339..397W
by	WILLOTT C.J. , SIMPSON C., ALMAINI O., MANNERS J.C., JOHNSON O., LAWRENCE A., DUNLOP J.S., IVISON R.J., RAWLINGS S., GONZALEZ-SOLARES E., PEREZ-FOURNON I., SERJEANT S., OLIVER S.J., ROCHE N.D., MANN R.G., ROWAN-ROBINSON M.
	Mon. Not. R. Astron. Soc., 339, 397-409 (2003)
	Obscured active galactic nuclei from the ELAIS Deep X-ray Survey.
o	Table 1: <CXOEN2 JHHMMSS.s+DDMMSS> N=3.
Ref:	=2003MNRAS.343..293M
by	MANNERS J.C. , JOHNSON O., ALMAINI O., WILLOTT C.J., GONZALEZ-SOLARES E., LAWRENCE A., MANN R.G., PEREZ-FOURNON I., DUNLOP J.S., McMAHON R.G., OLIVER S.J., ROWAN-ROBINSON M., SERJEANT S.
	Mon. Not. R. Astron. Soc., 343, 293-305 (2003)
	The ELAIS deep X-ray survey - I. Chandra source catalogue and first results.
o	Table 1: <[MJA2003] N1-NNN> N=130 among (Nos N1-1 to N1-149) = <CXOEN1 JHHMMSS.s+DDMMSS> N=130. Table 2: <[MJA2003] N2-NNN> N=103 among (Nos N2-1 to N2-114) = <CXOEN2 JHHMMSS.s+DDMMSS> N=103.
=E=	Catalogue in electronic form as J/MNRAS/343/293
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOGBA
CXOGBA	(Chandra X-ray Observatory, Gilmour+Best+Almaini)
Write:	<<CXOGBA JHHMMSS.s+DDMMSS>>
N:	about 8000
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	In preparation. An analysis of the point source distributions in Chandra archival observations of around about 120 galaxy clusters. (The source list includes far more faint sources than those detected by the Chandra archival surveys). Positions, count rates, detection significance and hardness ratio are given for each point source. See www.roe.ac.uk/∼red for the full catalogue.
Ref:	=2009MNRAS.392.1509G
by	GILMOUR R. , BEST P., ALMAINI O.
	Mon. Not. R. Astron. Soc., 392, 1509-1531 (2009)
	The distribution of active galactic nuclei in a large sample of galaxy clusters.
o	Table 4: <CXOGBA JHHMMSS.s+DDMMSS> N~9500.
=E=	Catalogue in electronic form as J/MNRAS/392/1509
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOGBS
CXOGBS	(Chandra X-ray Observatory Galactic Bulge Survey)
Write:	<<CXOGBS JHHMMSS.s+DDMMSS>>
N:	1234+424
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	The source list comes from the Galactic Bulge Survey, a mosaic of Chandra observations of two strips of 6 square degrees each. http://www.sron.nl/~peterj/gbs/
Ref:	=2011ApJS..194...18J
by	JONKER P.G. , BASSA C.G., NELEMANS G., STEEGHS D., TORRES M.A.P., MACCARONE T.J., HYNES R.I., GREISS S., CLEM J., DIEBALL A., MIKLES V.J., BRITT C.T., GOSSEN L., COLLAZZI A.C., WIJNANDS R., IN'T ZAND J.J.M., MENDEZ M., REA N., KUULKERS E., RATTI E.M., VAN HAAFTEN L.M., HEINKE C., OZEL F., GROOT P.J., VERBUNT F.
	Astrophys. J., Suppl. Ser., 194, 18 (2011)
	The Galactic Bulge Survey: outline and X-ray observations.
o	Table 3, col(1): <CXOGBS JHHMMSS.s+DDMMSS> N=1234 = Table 3, col(2): <[JBN2011] NNNN> (Nos 1-1234).
Ref:	=arXiv:1312.3192
Ref:	=2014ApJS..210...18J
by	JONKER P.G. , TORRES M.A.P., HYNES R.I., MACCARONE T.J., STEEGHS D., GREISS S., BRITT C.T., WU J., JOHNSON C.B., NELEMANS G., HEINKE C.
	Astrophys. J., Suppl. Ser., 210, 18 (2014)
	The Galactic Bulge Survey: completion of the X-ray survey observations.
o	Table 1, col(1): <CXOGBS JHHMMSS.s+DDMMSS> N=424 added, Table 1, col(2): <[JTH2014] CXBNNN> (Nos CXB1-CXB424). SRON, Netherlands Institute for Space Research
=E=	Catalogue in electronic form as J/ApJS/194/18
=E=	Catalogue in electronic form as J/ApJS/210/18
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOGC
CXOGC	(Chandra X-ray Observatory, Galactic Center)= (CXOUGC) = (CXOGCR)
Write:	<<CXOGC JHHMMSS.s+DDMMSS>>
N:	9017
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	The Chandra X-ray Observatory Galactic Center (CXOGC) project is an on-going, multi-year survey of X-ray sources in the Galactic Center from deep observations with the ACIS instrument on the Chandra X-ray Observatory. The first-year's observation was centered near the radio position of Sagittarius A*, the compact nonthermal radio-source at the dynamical center of our Galaxy thought to be powered by matter accreting onto a supermassive black hole. The deep imaging observation detected 150-200 X-ray sources in the 0.5-7 keV passband. Several hundred more sources will be detected as we perform deeper exposures of the Galactic Center with Chandra in the coming years. The ACIS-I field of view is 17-arcmin x17-arcmin. , MIT Center for Space Research. 2009ApJS..181..110M: updated catalog which incorporates and supersedes the previous catalogs.
in source:	NAME Gal Center
Ref:	=2002PASP..114....1W
by	WEISSKOPF M.C. , BRINKMAN B., CANIZARES C., GARMIRE G., MURRAY S., VAN SPEYBROECK L.P.
	Publ. Astron. Soc. Pac., 114, 1-24 (2002)
	An overview of the performance and scientific results from the Chandra X-ray observatory. (Invited review).
o	Fig.14: <CXOGC JHHMMSS.s-DDMMSS> N=2.
Ref:	=2003ApJ...589..225M
by	MUNO M.P. , BAGANOFF F.K., BAUTZ M.W., BRANDT W.N., BROOS P.S., FEIGELSON E.D., GARMIRE G.P., MORRIS M.R., RICKER G.R., TOWNSLEY L.K.
	Astrophys. J., 589, 225-241 (2003)
	A deep Chandra catalog of X-ray point sources toward the Galactic Center.
o	Catalog: <CXOGC JHHMMSS.s-DDMMSS> N=2357.
Ref:	=2009ApJS..181..110M
by	MUNO M.P. , BAUER F.E., BAGANOFF F.K., BANDYOPADHYAY R.M., BOWER G.C., BRANDT W.N., BROOS P.S., COTERA A., EIKENBERRY S.S., GARMIRE G.P., HYMAN S.D., KASSIM N.E., LANG C.C., LAZIO T.J.W., LAW C., MAUERHAN J.C., MORRIS M.R., NAGATA T., NISHIYAMA S., PARK S., RAMIREZ S.V., STOLOVY S.R., WIJNANDS R., WANG Q.D., WANG Z., YUSEF-ZADEH F.
	Astrophys. J., Suppl. Ser., 181, 110-128 (2009)
	A catalog of X-ray point sources from two megaseconds of Chandra observations of the Galactic center.
o	Table 2, col(1): numbering NNNN not used in SIMBAD.
o	Table 1: <GCS NN> (Nos 16-30) added. Table 2, col(2): <CXOGC JHHMMSS.s+DDMMSS> N=9017.
=E=	Catalogue in electronic form as J/ApJ/589/225
=E=	Catalogue in electronic form as <J/ApJS/181/110/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOGCR
CXOGCR	(Chandra X-ray Observatory, Galactic Center Region)
*****	Avoid the usage of CXOGCR, prefer CXOGC
Origin	of the Acronym: L (2005ApJ...634L..45C)
Details on Acronym: CXOGCS
CXOGCS	(Chandra X-ray Observatory, Galactic Center Survey)= (CXGCS)
Write:	<<CXOGCS JHHMMSS.s+DDMMSS>> <<CXOGCS JHHMMSS.ss+DDMMSS.s>>
N:	about 1000
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	This first large-scale Chandra survey of the Galactic Center region consists of 30 spatially-overlapped observations with exposure of about 11 ksec each. All these observations were taken in July, 2001. The arc-second spatial resolution and sensitivity of this survey is more detailed and complete by nearly two orders of magnitude than previous imaging in the 1-10 keV range. The survey allows, for the first time, a clean separation of the diffuse and point-like components of the X-ray emission, leading to a comprehensive characterization of high-energy activities in the region. We have detected about 1000 X-ray sources, compared to about two dozen previously known. See also [WDL2006].
in source:	NAME Gal Center
Ref:	=2006MNRAS.371...38W
by	WANG Q.D. , DONG H., LANG C.
	Mon. Not. R. Astron. Soc., 371, 38-54 (2006)
	The interplay between star formation and the nuclear environment of our Galaxy: deep X-ray observations of the Galactic centre Arches and Quintuplet clusters.
o	Table 1, col(1): <[WDL2006] NNN> (Nos 1-244) = Table 1, col(2): <CXOGCS JHHMMSS.ss+DDMMSS.s> N=244. Fig.2, Table 2: <[YLW2002] AN> (No. A6) added, <[LY2004] QXN> (No. QX5) added.
Ref:	=2006ApJS..165..173M
by	MUNO M.P. , BAUER F.E., BANDYOPADHYAY R.M., WANG Q.D.
	Astrophys. J., Suppl. Ser., 165, 173-187 (2006)
	A Chandra catalog of X-ray sources in the central 150 pc of the galaxy.
o	Table 2: <CXOGCS JHHMMSS.s+DDMMSS> N=1352.
=E=	Catalogue in electronic form as J/MNRAS/371/38
=E=	Catalogue in electronic form as J/ApJS/165/173
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOGlb
CXOGlb	(Chandra X-ray Observatory, GCl source)
Write:	<<CXOGlb JHHMMSS.s+DDMMSS>>
N:	4+9+300+50+14+1+61
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	X-ray sources discovered in globular clusters with Chandra X-ray observatory, expected to be cataclysmic variables, millisecond pulsars, low-mass x-ray binaries, and main sequence binaries such as BY Draconis binaries. Over 100 discovered in 47 Tucanae, 3 new sources in NGC 6652, more than 10 in NGC 6397, 50 in Cl Terzan 5.
in source:	NGC 104 = 47 Tuc
in source:	NGC 6652
in source:	NGC 6397
in source:	Cl Terzan 5
in source:	NGC 6388
in source:	NGC 6440
in source:	Cl Terzan 1
Ref:	=2001ApJ...562..363H
by	HEINKE C.O. , EDMONDS P.D., GRINDLAY J.E.
	Astrophys. J., 562, 363-367 (2001)
	Identification of the low-mass X-ray binary and faint X-ray sources in NGC 6652.
o	Table 1: <[HEG2001] A> (Nos A-D) = <CXOGlb JHHMMSS.s+DDMMSS> N=4.
Ref:	=2003ApJ...590..809H
by	HEINKE C.O. , EDMONDS P.D., GRINDLAY J.E., LLOYD D.A., COHN H.N., LUGGER P.M.
	Astrophys. J., 590, 809-821 (2003)
	A Chandra X-ray study of the dense globular cluster Terzan 5.
o	Fig.2, Table 1, col(2): <[HEG2003] WNN> (Nos W2-W10) = Table 1, col(1): <CXOGlb JHHMMSS.s+DDMMSS> N=9, <[HEG2003] Star N> (Nos 1-2).
o	p.811: source S2 of Johnston + 1995 is EQ J174734.4-244558 in SIMBAD.
Ref:	=2005ApJ...625..796H
by	HEINKE C.O. , GRINDLAY J.E., EDMONDS P.D., COHN H.N., LUGGER P.M., CAMILO F., BOGDANOV S., FREIRE P.C.
	Astrophys. J., 625, 796-824 (2005)
	A deep Chandra survey of the globular cluster 47 Tucanae: catalog of point sources.
o	Table 2: <[GHE2001] WNNN> N=180 added among (Nos W113-W351). Table 2: <CXOGlb JHHMMSS.s+DDMMSS> N=300.
Ref:	=2006ApJ...651.1098H
by	HEINKE C.O. , WIJNANDS R., COHN H.N., LUGGER P.M., GRINDLAY J.E., POOLEY D., LEWIN W.H.G.
	Astrophys. J., 651, 1098-1111 (2006)
	Faint X-ray sources in the globular cluster Terzan 5.
o	Table 1, col(1): <[HWC2006] CX NN> (Nos 1-50) = Table 1, col(2): <CXOGlb JHHMMSS.s+DDMMSS> N=50.
Ref:	=2006MNRAS.369..407C
by	CACKETT E.M. , WIJNANDS R., HEINKE C.O., POOLEY D., LEWIN W.H.G., GRINDLAY J.E., EDMONDS P.D., JONKER P.G., MILLER J.M.
	Mon. Not. R. Astron. Soc., 369, 407-415 (2006)
	A Chandra X-ray observation of the globular cluster Terzan 1.
o	Table 1, col(2): <[CWH2006] CXNN> (Nos CX1-CX14) = Table 1, col(1): <CXOGlb JHHMMSS.s+DDMMSS> N=14.
Ref:	=2010ApJ...714..894H
by	HEINKE C.O. , ALTAMIRANO D., COHN H.N., LUGGER P.M., BUDAC S.A., SERVILLAT M., LINARES M., STROHMAYER T.E., MARKWARDT C.B., WIJNANDS R., SWANK J.H., KNIGGE C., BAILYN C., GRINDLAY J.E.
	Astrophys. J., 714, 894-903 (2010)
	Discovery of a second transient low-mass X-ray binary in the globular cluster NGC 6440.
o	<[HAC2010] NGC 6440 X-2> N=1 = <CXOGlb JHHMMSS.s+DDMMSS> N=1.
Ref:	=2012ApJ...756..147M
by	MAXWELL J.E. , LUGGER P.M., COHN H.N., HEINKE C.O., GRINDLAY J.E., BUDAC S.A., DRUKIER G.A., BAILYN C.D.
	Astrophys. J., 756, 147 (2012)
	X-ray binaries in the ultrahigh encounter rate globular cluster NGC 6388.
o	Table 4, col(1): <[MLC2012] CX NN> (Nos 1-61) = Table 4, col(2): <CXOGlb JHHMMSS.s+DDMMSS> N=61.
=E=	Catalogue in electronic form as J/ApJ/625/796
=E=	Catalogue in electronic form as J/ApJ/651/1098
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOGMP
CXOGMP	(Chandra X-ray Observatory, Garcia+Murray+Primini)
Write:	<<CXOGMP JHHMMSS.s+DDMMSS>>
N:	about 100
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Point X-ray sources found in M31 as part of the guaranteed time project for the Chandra X-ray Observatory. N about 100. 1st ref.: 2000ApJ...537L..23G, N=6 objects.
in source:	M 31 = NGC 224
Ref:	=2000ApJ...537L..23G
by	GARCIA M.R. , MURRAY S.S., PRIMINI F.A., FORMAN W.R., McCLINTOCK J.E., JONES C.
	Astrophys. J., 537, 23-26 (2000)
	A first look at the nuclear region of M31 with Chandra.
o	Table 1, text: <CXOGMP JHHMMSS.s+DDMMSS> N=6.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOGNC
CXOGNC	(Chandra X-ray Observatory Great Nebula in Carina)
Write:	<<CXOGNC JHHMMSS.ss+DDMMSS.s>>
N:	about 14000
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	The Chandra Carina Complex Project.
Ref:	=2011ApJS..194....2B
by	BROOS P.S. , TOWNSLEY L.K., FEIGELSON E.D., GETMAN K.V., GARMIRE G.P., PREIBISCH T., SMITH N., BABLER B.L., HODGKIN S., INDEBETOUW R., IRWIN M., KING R.R., LEWIS J., MAJEWSKI S.R., McCAUGHREAN M.J., MEADE M.R., ZINNECKER H.
	Astrophys. J., Suppl. Ser., 194, 2 (2011)
	A catalog of Chandra X-ray sources in the Carina nebula.
o	Tables 1, 6: <CXOGNC JHHMMSS.ss+DDMMSS.s> N=14369. Pennsylvania State University
=E=	Catalogue in electronic form as <J/ApJS/194/2/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOGPE
CXOGPE	(Chandra X-ray Observatory, Galactic Plane, Ebisawa+)
Write:	<<CXOGPE JHHMMSS.s+DDMMSS>>
N:	274
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	New X-ray sources detected in two Chandra deep observations (each 100 ksec) on the Galactic Plane region at around (l,b) about (28.5,-0.1). Total surveyed area is about 250 arcmin(2). See also [ETP2005].
Ref:	=2005ApJ...635..214E
by	EBISAWA K. , TSUJIMOTO M., PAIZIS A., HAMAGUCHI K., BAMBA A., CUTRI R., KANEDA H., MAEDA Y., SATO G., SENDA A., UENO M., YAMAUCHI S., BECKMANN V., COURVOISIER T.J.-L., DUBATH P., NISHIHARA E.
	Astrophys. J., 635, 214-242 (2005)
	Chandra deep X-ray observation of a typical Galactic plane region and near-infrared identification.
o	Fig. 12 : CXOU J184357-035441 (incomplete format) = EQ J184357-035441 in SIMBAD
o	Table 1: <CXOGPE JHHMMSS.s+DDMMSS> N=274 = <[ETP2005] X NNN> (Nos 1-274). Table 2: <[ETP2005] NIR NNNNN> (Nos 1-32398).
=E=	Catalogue in electronic form as J/ApJ/635/214
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOGSG
CXOGSG	(sources named by Galaxy Structure Group (NAOC), using Chandra X-ray Observatory data)
Write:	<<CXOGSG JHHMMSS.s+DDMMSS>>
N:	217828
Object:	(X)
Note:	The Chandra archival data is a valuable resource for various studies on different topics of X-ray astronomy. We utilize this wealth and present a uniformly processed data set, which can be used to address a wide range of scientific questions by a broad-based group of scientists. The data analysis procedures are applied to 10,029 ACIS observations, and produce about 218,000 distinct X-ray sources.
Ref:	=2016ApJS..224...40W
by	WANG S. , LIU J., QIU Y., BAI Y., YANG H., GUO J., ZHANG P.
	Astrophys. J., Suppl. Ser., 224, 40-40 (2016)
	CHANDRA ACIS survey of X-ray point sources: the source catalog.
o	Tables 3-5: <CXOGSG JHHMMSS.s+DDMMSS> N=217828. National Astronomical Observatories, Chinese Academy of Sciences
=E=	Catalogue in electronic form as <J/ApJS/224/40/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOGWS
CXOGWS	(CXO, Groth Westphal Survey)
Write:	<<CXOGWS JHHMMSS.s+DDMMSS>>
N:	158
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra X-ray survey of the Groth Strip. The survey has been extended to the region known as the Extended Groth Strip: see CXOEGS. See also [NLA2005].
in source:	NAME Groth-Westphal Strip
Ref:	=2005MNRAS.356..568N
by	NANDRA K. , LAIRD E.S., ADELBERGER K., GARDNER J.P., MUSHOTZKY R.F., RHODES J., STEIDEL C.C., TEPLITZ H.I., ARNAUD K.A.
	Mon. Not. R. Astron. Soc., 356, 568-586 (2005)
	A deep Chandra survey of the Groth Strip - I. The X-ray data.
o	Table 3, col(1): <[NLA2005] cNNNN> (Nos c1-c158) = Table 3, col(2): <CXOGWS JHHMMSS.s+DDMMSS> N=158. Table A1, col(1): <[NLA2005] aNNN> N=21 among (Nos a6-a142) = Table A1, col(2): <CXOEN1 JHHMMSS.s+DDMMSS> N=21 added. Table A2, col(1): <[NLA2005] fNNN> N=75 among (Nos f9-f536) = Table A2, col(2): <CXOHDFN JHHMMSS.s+DDMMSS> N=75 added.
=E=	Catalogue in electronic form as J/MNRAS/356/568
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOHCD
CXOHCD	(CXO, Haggard+Cool+Davies)
Write:	<<CXOHCD JHHMMSS.ss+DDMMSS.s>>
N:	180
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Comprehensive catalog of the Chandra X-ray sources coincident with the galactic globular cluster Omega Centauri (NGC 5139). N=180 X-ray sources in the Chandra ACIS-I field of view, roughly 30 of which are associated with the cluster. Non-members are likely a combination of background AGN and foreground dMe (or other active) stars.
in source:	Ome Cen = NGC 5139
Auth.:	HAGGARD D.+
Ref:	=2009ApJ...697..224H
by	HAGGARD D. , COOL A.M., DAVIES M.B.
	Astrophys. J., 697, 224-236 (2009)
	A Chandra study of the Galactic globular cluster ω Centauri.
o	Table 1, col(1): <[HCD2009] NNNa> N=180 = Table 1, col(2): <CXOHCD JHHMMSS.ss+DDMMSS.s> N=180.
=E=	Catalogue in electronic form as <J/ApJ/697/224/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOHDFN
CXOHDFN	(Chandra X-ray Observatory, Hubble Deep Field North)
Write:	<<CXOHDFN JHHMMSS.s+DDMMSS>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of the HDFN. These sources were detected during the 1 million second Chandra Deep Field-North survey of the Hubble Deep Field-North area. This survey will be extended to a depth of 2 million seconds during 2001-2002. Please see http://www.astro.psu.edu/users/niel/hdf/hdf-chandra.html for more details. See also [HBG2001], [ABB2003], [NLA2005].
in source:	NAME HDFN
Ref:	=2000ApJ...541...49H
by	HORNSCHEMEIER A.E. , BRANDT W.N., GARMIRE G.P., SCHNEIDER D.P., BROOS P.S., TOWNSLEY L.K., BAUTZ M.W., BURROWS D.N., CHARTAS G., FEIGELSON E.D., GRIFFITHS R., LUMB D., NOUSEK J.A., SARGENT W.L.W.
	Astrophys. J., 541, 49-53 (2000)
	X-ray sources in the Hubble Deep Field detected by Chandra.
o	Table 1: <CXOHDFN JHHMMSS.s+DDMMSS> N=6.
Ref:	=2001ApJ...554..742H
by	HORNSCHEMEIER A.E. , BRANDT W.N., GARMIRE G.P., SCHNEIDER D.P., BARGER A.J., BROOS P.S., COWIE L.L., TOWNSLEY L.K., BAUTZ M.W., BURROWS D.N., CHARTAS G., FEIGELSON E.D., GRIFFITHS R.E., LUMB D., NOUSEK J.A., RAMSEY L.W., SARGENT W.L.W.
	Astrophys. J., 554, 742-777 (2001)
	The Chandra deep survey of the Hubble Deep Field-north area. II. Results from the Caltech faint field galaxy redshift survey area.
o	Table 4, col(1): <[HBG2001] NN> (Nos 1-82) = <CXOHDFN JHHMMSS.s+DDMMSS> N=82.
Ref:	=2001AJ....122.2156A
by	ALEXANDER D.M. , BRANDT W.N., HORNSCHEMEIER A.E., GARMIRE G.P., SCHNEIDER D.P., BAUER F.E., GRIFFITHS R.E.
	Astron. J., 122, 2156-2176 (2001)
	The Chandra Deep Field North survey. VI. The nature of the optically faint X-ray source population.
o	Table 1: <CXOHDFN JHHMMSS.s+DDMMSS> N=41 added.
Ref:	=2001AJ....122.2810B
by	BRANDT W.N. , ALEXANDER D.M., HORNSCHEMEIER A.E., GARMIRE G.P., SCHNEIDER D.P., BARGER A.J., BAUER F.E., BROOS P.S., COWIE L.L., TOWNSLEY L.K., BURROWS D.N., CHARTAS G., FEIGELSON E.D., GRIFFITHS R.E., NOUSEK J.A., SARGENT W.L.W.
	Astron. J., 122, 2810-2832 (2001)
	The Chandra Deep Field North survey. V. 1 Ms source catalogs.
o	p.2831 (end of. ch.3.3): F36397+1547 = [DSB2001] F36397-1547, F36421+1545 = [HPA2000] J123642.16+621545.2.
o	Table 3: <[BAH2001] NNN> (Nos 1-370) = <CXOHDFN JHHMMSS.s+DDMMSS> N=370. Table 6: <[BAH2001] SNN> (Nos S1-S11) = <CXOHDFN JHHMMSS.s+DDMMSS> N=11.
Ref:	=2005MNRAS.356..568N
by	NANDRA K. , LAIRD E.S., ADELBERGER K., GARDNER J.P., MUSHOTZKY R.F., RHODES J., STEIDEL C.C., TEPLITZ H.I., ARNAUD K.A.
	Mon. Not. R. Astron. Soc., 356, 568-586 (2005)
	A deep Chandra survey of the Groth Strip - I. The X-ray data.
o	Table 3, col(1): <[NLA2005] cNNNN> (Nos c1-c158) = Table 3, col(2): <CXOGWS JHHMMSS.s+DDMMSS> N=158. Table A1, col(1): <[NLA2005] aNNN> N=21 among (Nos a6-a142) = Table A1, col(2): <CXOEN1 JHHMMSS.s+DDMMSS> N=21 added. Table A2, col(1): <[NLA2005] fNNN> N=75 among (Nos f9-f536) = Table A2, col(2): <CXOHDFN JHHMMSS.s+DDMMSS> N=75 added.
=E=	Catalogue in electronic form as J/ApJ/554/742
=E=	Catalogue in electronic form as J/AJ/122/2810
=E=	Catalogue in electronic form as J/MNRAS/356/568
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOHDFS
CXOHDFS	(Chandra X-ray Observatory, Hubble Deep Field South)
Write:	<<CXOHDFS JHHMMSS.s+DDMMSS>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of the HDFS.
in source:	NAME HDFS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CXOIC1396A
CXOIC1396A	(Chandra X-ray Observatory, IC1396A)
Write:	<<CXOIC1396A JHHMMSS.ss+DDMMSS.s>>
N:	415
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS observations of N=415 X-ray sources in IC 1396A. See also [GFS2012].
in source:	IC 1396A
Ref:	=2012MNRAS.426.2917G
by	GETMAN K.V. , FEIGELSON E.D., SICILIA-AGUILAR A., BROOS P.S., KUHN M.A., GARMIRE G.P.
	Mon. Not. R. Astron. Soc., 426, 2917-2943 (2012)
	The Elephant Trunk Nebula and the Trumpler 37 cluster: contribution of triggered star formation to the total population of an HII region.
o	Tables 1-3: <[GFS2012] NNN> (Nos 1-415) = Table 1, col(2): <CXOIC1396A JHHMMSS.ss+DDMMSS.s> N=415. Table 4: <[GFS2012] IR NN> (Nos 1-42). Fig. 13: <[GFS2012] GN> (Nos G1-G7), <[GFS2012] G1267> N=1.
=E=	Catalogue in electronic form as <J/MNRAS/426/2917/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CXOKM101
CXOKM101	(Chandra X-ray Observatory catalogue, Kuntz, M101)
Write:	<<CXOKM101 JHHMMSS.s+DDMMSS>>
N:	about 300
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	In preparation. Comprehensive catalogue of sources detected by Chandra in a total of 10 fields in the nearby spiral galaxy M101. This catalogue will be released incrementally as analysis is extended from the central region (chip ACIS-S3) to the other useful chips (particularly chip ACIS-S2). This catalogue will supersede that in Pence et al. 2001, 2001ApJ...561..189P, [PSM2001]. The coordinate frame will be referenced to the HST guide star frame.
Auth.:	KUNTZ K.D.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOKMZ
CXOKMZ	(CXO, Kundu+Maccarone+Zepf)
Write:	<<CXOKMZ JHHMMSS.s+DDMMSS>>
N:	175+86+71+141+165
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS data of five early-type galaxies. See also [KMZ2007]
in source:	NGC 1399
in source:	NGC 3115
in source:	NGC 3379
in source:	NGC 4594
in source:	NGC 4649
Ref:	=2007ApJ...662..525K
by	KUNDU A. , MACCARONE T.J., ZEPF S.E.
	Astrophys. J., 662, 525-543 (2007)
	Probing the formation of low-mass X-ray binaries in globular clusters and the field.
o	Tables 2,5,8,11,14, col(1): <[KMZ2007] NGC NNNN X NNN> = Tables 2,5,8,11,14, col(2): <CXOKMZ JHHMMSS.s+DDMMSS> N=175+86+71+141+165. Tables 3,6,9,12,15: <[KMZ2007] NGC NNNN GC NNN> N=554+133+61+193+418.
=E=	Catalogue in electronic form as J/ApJ/662/525
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CXOLALA1
CXOLALA1	(Chandra, Large Array Lyman-Alpha survey, No. 1)
Write:	<<CXOLALA1 JHHMMSS.s+DDMMSS>>
N:	168
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of the Large Array Lyman-Alpha survey (LALA) Bootes field with the ACIS-I. See also [WMR2004].
in source:	NAME Bootes Field
Ref:	=2004AJ....127..213W
by	WANG J.X. , MALHOTRA S., RHOADS J.E., BROWN M.J.I., DEY A., HECKMAN T.M., JANNUZI B.T., NORMAN C.A., TIEDE G.P., TOZZI P.
	Astron. J., 127, 213-229 (2004)
	The 172 ks Chandra exposure of the LALA Bootes field: X-ray source catalog.
o	Table 1. col(1): <[WMR2004] NNN> (Nos 1-168) = Table 1. col(2): <CXOLALA1 JHHMMSS.s+DDMMSS> N=168.
=E=	Catalogue in electronic form as J/AJ/127/213
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CXOLALA2
CXOLALA2	(Chandra, Large Array Lyman-Alpha survey, No. 2)
Write:	<<CXOLALA2 JHHMMSS.s+DDMMSS.s>>
N:	188
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS observations of the Large Array Lyman-Alpha survey (LALA) Cetus field. See also [WZM2007].
in source:	NAME Cetus Field
Ref:	=2007ApJ...669..765W
by	WANG J.X. , ZHENG Z.Y., MALHOTRA S., FINKELSTEIN S.L., RHOADS J.E., NORMAN C.A., HECKMAN T.M.
	Astrophys. J., 669, 765-775 (2007)
	Chandra X-ray sources in the LALA Cetus field.
o	Table 1, col(2): The format of CXOLALA2 objects is always JHHMMSS.s+DDMMSS.s, when the seconds of declination are written 0S.s, the '0' has been omitted.
o	Table 1, col(1): <[WZM2007] NNN> (Nos 1-188) = Table 1, col(2): <CXOLALA2 JHHMMSS.s+DDMMSS.s> N=188.
=E=	Catalogue in electronic form as J/ApJ/669/765
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CXOLV
CXOLV	(Chandra X-ray Observatory Local Volume Survey)
Write:	<<CXOLV JHHMMSS.s+DDMMSS>>
N:	about 700
Object:	Poss. LMXB + Poss. HMXB (SIMBAD class: X = X-ray Source)
Note:	The Chandra Local Volume Survey is a deep, volume-limited X-ray survey of five nearby galaxies (NGC 55, NGC 300, NGC 404, NGC 2403, and NGC 4214) with matched Hubble Space Telescope observations down to an absolute V-band magnitude of ∼0. These galaxies contain ∼99% of the extragalactic stellar mass and 90% of the recent star formation outside of the Local Group out to a distance of 3.3 Mpc and span a range of stellar masses, morphologies, and metallicities. We are generating X-ray point source catalogs for each galaxy and correlating the properties of the X-ray binary populations (such as the X-ray luminosity function) to the host galaxy's star formation rate, thereby providing an observational test of theoretical predictions. We will first be publishing the X-ray source catalog of NGC 300, with additional papers on the remaining four galaxies forthcoming. Each galaxy hosts 70-190 X-ray point sources, for a total survey sample of up to ∼700 X-ray sources requiring designations.
in source:	NGC 55
in source:	NGC 300
in source:	NGC 404
in source:	NGC 2403
in source:	NGC 4214
Auth.:	Breanna Binder University of Washington
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOLV
CXOLV	(Chandra X-ray Observatory Local Volume Survey)
Write:	<<CXOLV JHHMMSS.ss+DDMMSS.s>>
N:	95+74+967
Object:	Poss. LMXB + Poss. HMXB (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS observations of N=95+72+460 X-ray point sources as part of the Chandra Local Volume Survey. See also [BWE2012], [BWE2013] and [BWE2015].
in source:	NGC 55
in source:	NGC 300
in source:	NGC 404
in source:	NGC 2403
in source:	NGC 4214
Ref:	=2012ApJ...758...15B
by	BINDER B. , WILLIAMS B.F., ERACLEOUS M., GAETZ T.J., PLUCINSKY P.P., SKILLMAN E.D., DALCANTON J.J., ANDERSON S.F., WEISZ D.R., KONG A.K.H.
	Astrophys. J., 758, 15 (2012)
	The Chandra Local Volume Survey: the X-ray point-source catalog of NGC 300.
o	Tables 4-7, Col(ID): <CXOLV JHHMMSS.ss+DDMMSS.s> N=95 = Tables 4-7, Col(Seq): <[BWE2012] NGC 300 NN> (Nos 1-95).
Ref:	=2013ApJ...763..128B
by	BINDER B. , WILLIAMS B.F., ERACLEOUS M., GAETZ T.J., KONG A.K.H., SKILLMAN E.D., WEISZ D.R.
	Astrophys. J., 763, 128 (2013)
	The Chandra local volume survey: the X-ray point-source population of NGC 404.
o	Tables 3-6, 10, 13, Col(ID): <CXOLV JHHMMSS.ss+DDMMSS.s> N=74 = Tables 3-6, 10, 13, Col(Seq): <[BWE2013] NGC 404 NN> (Nos 1-74).
Ref:	=2015AJ....150...94B
by	BINDER B. , WILLIAMS B.F., ERACLEOUS M., PLUCINSKY P.P., GAETZ T.J., ANDERSON S.F., SKILLMAN E.D., DALCANTON J.J., KONG A.K.H., WEISZ D.R.
	Astron. J., 150, 94 (2015)
	The Chandra Local Volume Survey. I. The X-ray point source populations of NGC 55, NGC 2403, and NGC 4214.
o	Table 5: <CXOLV JHHMMSS.ss+DDMMSS.s> N=967. Tables 8, 20 : <[BWE2015] NGC NNNN NNN> N=460. University of Washington
=E=	Catalogue in electronic form as J/ApJ/758/15
=E=	Catalogue in electronic form as J/ApJ/763/128
=E=	Catalogue in electronic form as J/AJ/150/94
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CXOM20
CXOM20	(Chandra X-ray Observatory, M 20)
Write:	<<CXOM20 JHHMMSS.ss+DDMMSS.s>>
N:	304
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra X-ray Observatory observations of the Trifid Nebula. See also the other designation [RRC2004] for the same objects.
in source:	M 20 = Trifid Nebula
Ref:	=2004ApJ...607..904R
by	RHO J. , RAMIREZ S.V., CORCORAN M.F., HAMAGUCHI K., LEFLOCH B.
	Astrophys. J., 607, 904-912 (2004)
	Chandra observation of the Trifid nebula: X-ray emission from the O star complex and actively forming pre-main-sequence stars.
o	Table 1: <[RRC2004] NNN> (Nos 1-304) = <CXOM20 JHHMMSS.ss+DDMMSS.s> N=304.
=E=	Catalogue in electronic form as J/ApJ/607/904
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CXOM31
CXOM31	(Chandra X-ray Observatory, M 31)
Write:	<<CXOM31 JHHMMSS.s+DDMMSS>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra X-ray sources in the central region of M 31. See also [KGP2002]. There are many Chandra observing programs on M31. One is a 'monitoring' program surveying M31 about one month. There are several other deeper, but smaller FOV programs targeting specific sections of the galaxy. The naming convention is used for the first time in 2002ApJ...577..738.
in source:	M 31 = NGC 224
Ref:	=2002ApJ...577..738K
by	KONG A.K.H. , GARCIA M.R., PRIMINI F.A., MURRAY S.S., DI STEFANO R., McCLINTOCK J.E.
	Astrophys. J., 577, 738-756 (2002)
	X-ray point sources in the central region of M31 as seen by Chandra.
o	Table 4: mita NNN = [M93b] NNN in SIMBAD.
o	Table 2, col(1): <[KGP2002] rN-NNN> (Nos r1-1 to r1-33, r2-1 to r2-59, r3-1 to r3-112) = Table 2, col(2): <CXOM31 JHHMMSS.s+DDMMSS> N=204.
Ref:	=2002ApJ...570..618D
by	DI STEFANO R. , KONG A.K.H., GARCIA M.R., BARMBY P., GREINER J., MURRAY S.S., PRIMINI F.A.
	Astrophys. J., 570, 618-636 (2002)
	Bright X-ray sources in M31 globular clusters.
o	Table 3: ID Mita = [M93b] NNN in SIMBAD. Table 3 note e : Source 25 is a misprint for Source 24.
o	Table 3: <[DKG2002] NN> (Nos 1-28) = <CXOM31 JHHMMSS.s+DDMMSS> N=28.
Ref:	=2004ApJ...609..735W
by	WILLIAMS B.F. , GARCIA M.R., KONG A.K.H., PRIMINI F.A., KING A.R., DI STEFANO R., MURRAY S.S.
	Astrophys. J., 609, 735-754 (2004)
	A synoptic X-ray study of M31 with the Chandra high resolution camera.
o	Table 2: <[KGP2002] r1-NN> N=2 added, <[KGP2002] r2-NN> N=4 added, <[KGP2002] r3-NNN> N=3 added, <[KGP2002] s1-NN> N=27 among 85, <[KGP2002] s2-NN> N=1 (No. 63), <[KGP2002] n1-NN> N=15 among 85. Table 2: <CXOM31 JHHMMSS.s+DDMMSS> N=55 added.
Ref:	=2004ApJ...610..247D
by	DI STEFANO R. , KONG A.K.H., GREINER J., PRIMINI F.A., GARCIA M.R., BARMBY P., MASSEY P., HODGE P.W., WILLIAMS B.F., MURRAY S.S., CURRY S., RUSSO T.A.
	Astrophys. J., 610, 247-260 (2004)
	Supersoft X-ray sources in M31. I. A Chandra survey and an extension to quasi-soft sources.
o	Table 1: <[KGP2002] r2-NN> N=5 added, <[KGP2002] s1-NN> N=7 added, <[KGP2002] s2-NN> N=9 added, <[KGP2002] n1-NN> N=10 added. Table 1: <CXOM31 JHHMMSS.s+DDMMSS> N=31 added.
=E=	Catalogue in electronic form as J/ApJ/577/738
=E=	Catalogue in electronic form as J/ApJ/609/735
=E=	Catalogue in electronic form as J/ApJ/610/247
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOM32
CXOM32	(Chandra X-ray Observatory, M 32)
Write:	<<CXOM32 JHHMMSS.s+DDMMSS>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra X-ray sources the center of M 32. See also [HTU2003].
in source:	M 32 = NGC 221
Ref:	=2003ApJ...589..783H
by	HO L.C. , TERASHIMA Y., ULVESTAD J.S.
	Astrophys. J., 589, 783-789 (2003)
	Detection of the ``Active'' nucleus of M32.
o	Table 1: <[HTU2003] X-N> (Nos X-1 to X-3) = <CXOM32 JHHMMSS.s+DDMMSS> N=3.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CXOM33
CXOM33	(Chandra X-ray Observatory, M 33)
Write:	<<CXOM33 JHHMMSS.ss+DDMMSS.s>>
N:	about 1000
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Very Large Project (VLP) with the Chandra X-ray Observatory to map out the inner regions of the M33 galaxy with a total of 1.4 Ms, comprised of seven 200 ks pointing at seven fields.
in source:	M 33 = NGC 598
Ref:	=2005AJ....130..539G
by	GHAVAMIAN P. , BLAIR W.P., LONG K.S., SASAKI M., GAETZ T.J., PLUCINSKY P.P.
	Astron. J., 130, 539-553 (2005)
	Revealing the supernova remnant population of M33 with Chandra.
o	CXOM33 J013350.5+303821.5 has been changed in CXOM33 J013350.49+303821.5 in the complete catalog of CXOM33 objects. M33 X-8 = [LDC81] 8.
o	Text: <CXOM33 JHHMMSS.ss+DDMMSS.s> N=2.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOM51
CXOM51	(Chandra, M 51)
Write:	<<CXOM51 JHHMMSS.s+DDMMSS>>
N:	84+12+17
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of sources in M 51 field.
in source:	M 51 = NGC 5194
Ref:	=2004ApJ...601..735T
by	TERASHIMA Y. , WILSON A.S.
	Astrophys. J., 601, 735-758 (2004)
	The luminous X-ray source population in M51 observed with Chandra.
o	Table 2: <[TW2004] NGC 5194 NN> (Nos 1-84) = <CXOM51 JHHMMSS.s+DDMMSS> N=84. Table 3: <[TW2004] NGC 5195 NN> (Nos 1-12) = <CXOM51 JHHMMSS.s+DDMMSS> N=12. Table 4: <[TW2004] Source NN> (Nos 1-17) = <CXOM51 JHHMMSS.s+DDMMSS> N=17.
=E=	Catalogue in electronic form as J/ApJ/601/735
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CXOM82
CXOM82	(Chandra X-ray Observatory, M 82)
Write:	<<CXOM82 JHHMMSS.s+DDMMSS>>
N:	24
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of M 82 starburst galaxy. N=7 objects are the same in both references, but with some slight difference in coordinates.
in source:	M 82 = NGC 3034
Ref:	=2000Sci...290.1325G
by	GRIFFITHS R.E. , PTAK A., FEIGELSON E.D., GARMIRE G., TOWNSLEY L., BRANDT W.N., SAMBRUNA R., BREGMAN J.N.
	Science, 290, 1325-1328 (2000)
	Hot plasma and black hole binaries in starburst galaxy M82.
o	Table 1: <CXOM82 JHHMMSS.s+DDMMSS> N=22.
Ref:	=2001ApJ...547L..25M
by	MATSUMOTO H. , TSURU T.G., KOYAMA K., AWAKI H., CANIZARES C.R., KAWAI N., MATSUSHITA S., KAWABE R.
	Astrophys. J., 547, 25-28 (2001)
	Discovery of a luminous, variable, off-center source in the nucleus of M82 with the Chandra high-resolution camera.
o	Table 1, col(2): 7 objects CXOM82 are the same as in 2000Sci...290.1325G, but with some slight difference in coordinates.
o	Table 1: <[MTK2001b] N> (Nos 1-9) = <CXOM82 JHHMMSS.s+DDMMSS> N=2 added.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CXOMKZ
CXOMKZ	(Chandra X-ray Observatory, Maccarone+Kundu+Zepf)
Write:	<<CXOMKZ JHHMMSSs+DDMMSS>>
N:	148
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of NGC 4472. See also [MKZ2003].
in source:	NGC 4472 = M 49
Ref:	=2003ApJ...586..814M
by	MACCARONE T.J. , KUNDU A., ZEPF S.E.
	Astrophys. J., 586, 814-825 (2003)
	The low-mass X-ray binary-globular connection. II. NGC 4472 X-ray source properties and source catalogs.
o	Table 1: <[MKZ2003] XID NNN> (Nos 1-148) = <CXOMKZ JHHMMSSs+DDMMSS> N=148. Table 2: <[MKZ2003] OID NNNN> (Nos 1-1102).
=E=	Catalogue in electronic form as J/ApJ/586/814
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CXOMP
CXOMP	(Chandra Multi-wavelength Project)
Write:	<<CXOMP JHHMMSS.s+DDMMSS>>
N:	about 6800
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Survey of serendipitous X-ray sources in the Chandra X-ray Observatory archival data. These are being followed-up with optical imaging and spectroscopy in order to identify and classify the sources into their various types. The authors (Wilkes+, ) expect a final sample of around 4000 sources, 70/100 of which will be active galactic nuclei.
Ref:	=2004ApJS..150...19K
by	KIM D.-W. , CAMERON R.A., DRAKE J.J., EVANS N.R., FREEMAN P., GAETZ T.J., GHOSH H., GREEN P.J., HARNDEN F.R.Jr, KAROVSKA M., KASHYAP V., MAKSYM P.W., RATZLAFF P.W., SCHLEGEL E.M., SILVERMAN J.D., TANANBAUM H.D., VIKHLININ A.A., WILKES B.J., GRIMES J.P.
	Astrophys. J., Suppl. Ser., 150, 19-None (2004)
	Chandra multiwavelength project. I. First X-ray source catalog.
o	Table 7: <CXOMP JHHMMSS.s+DDMMSS> N=991.
Ref:	=2007ApJS..169..401K
by	KIM M. , KIM D.-W., WILKES B.J., GREEN P.J., KIM E., ANDERSON C.S., BARKHOUSE W.A., EVANS N.R., IVEZIC Z., KAROVSKA M., KASHYAP V.L., LEE M.G., MAKSYM P., MOSSMAN A.E., SILVERMAN J.D., TANANBAUM H.D.
	Astrophys. J., Suppl. Ser., 169, 401-429 (2007)
	Chandra multiwavelength project X-ray point source catalog.
o	Table 3: <CXOMP JHHMMSS.s+DDMMSS> N= about 6800.
=E=	Catalogue in electronic form as J/ApJS/150/19
=E=	Catalogue in electronic form as J/ApJS/169/401
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXONGC1333
CXONGC1333	(Chandra, NGC 1333)
Write:	<<CXONGC1333 JHHMMSS.s+DDMMSS>>
N:	109
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	The Chandra X-ray Observatory observed the NGC 1333 star forming region and detected several dozen X-ray emitting young stars. See also [GFT2002]
in source:	NGC 1333
Ref:	=2002ApJ...575..354G
by	GETMAN K.V. , FEIGELSON E.D., TOWNSLEY L., BALLY J., LADA C.J., REIPURTH B.
	Astrophys. J., 575, 354-377 (2002)
	Chandra study of young stellar objects in the NGC 1333 star-forming cloud.
o	Table 1, col(1): <[GFT2002] NNN> (Nos 1-109) = Table 1, col(2): <CXONGC1333 JHHMMSS.s+DDMMSS> N=109.
=E=	Catalogue in electronic form as J/ApJ/575/354
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXONGC3293
CXONGC3293	(Chandra X-ray sources in NGC 3293)
Write:	<<CXONGC3293 JHHMMSS.ss+DDMMSS.s>>
N:	1026
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	We performed a deep (70 ksec) X-ray observation of the young stellar cluster NGC 3293 with Chandra/ACIS and detected 1026 individual X-ray point sources.
Ref:	=2017A&A...605A..85P
by	PREIBISCH T. , FLAISCHLEN S., GACZKOWSKI B., TOWNSLEY L., BROOS P.
	Astron. Astrophys., 605A, 85-85 (2017)
	Chandra X-ray observation of the young stellar cluster NGC 3293 in the Carina Nebula Complex.
o	Table 1: <CXONGC3293 JHHMMSS.ss+DDMMSS.s> N=1026. Universitaets-Sternwarte Muenchen
=E=	Catalogue in electronic form as <J/A+A/605/A85/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOONC
CXOONC	(Chandra X-ray Observatory, Orion Nebula Cluster)
Write:	<<CXOONC JHHMMSS.s+DDMMSS>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	X-ray emitting young stars in the Orion Nebula region found with the Chandra X-ray Observatory. See also [GFB2000], [FBG2002].
in source:	NAME ONC
Ref:	=2000AJ....120.1426G
by	GARMIRE G. , FEIGELSON E.D., BROOS P., HILLENBRAND L.A., PRAVDO S.H., TOWNSLEY L., TSUBOI Y.
	Astron. J., 120, 1426-1435 (2000)
	Chandra X-ray observatory study of the Orion nebula cluster and BN/KL region.
o	Infrared source n = LBLS n, source radio D = GMR D
o	Table 1: <[GFB2000] ONC NNN> (Nos 1-973) = <CXOONC JHHMMSS.s+DDMMSS> N=973. Table 2: <[GFB2000] BN NN> (Nos 1-27) = <CXOONC JHHMMSS.s+DDMMSS> N=27.
Ref:	=2002ApJ...574..258F
by	FEIGELSON E.D. , BROOS P., GAFFNEY III J.A., GARMIRE G., HILLENBRAND L.A., PRAVDO S.H., TOWNSLEY L., TSUBOI Y.
	Astrophys. J., 574, 258-292 (2002)
	X-ray-emitting young stars in the Orion nebula.
o	Table 2: <[FBG2002] NNNN> (Nos 1-1075) = <CXOONC JHHMMSS.s+DDMMSS> N=1075.
=E=	Catalogue in electronic form as J/AJ/120/1426
=E=	Catalogue in electronic form as J/ApJ/574/258
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOP
CXOP	(Chandra X-ray Observatory, Pleiades)
Write:	<<CXOP JHHMMSS.s+DDMMSS>>
N:	99
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of the Pleiades.
in source:	NAME Pleiades
Ref:	=2002ApJ...578..486D
by	DANIEL K.J. , LINSKY J.L., GAGNE M.
	Astrophys. J., 578, 486-502 (2002)
	Chandra observations of the Pleiades open cluster: X-ray emission from late B- to early F-type binaries.
o	Table 1: <CXOP JHHMMSS.s+DDMMSS> N=99.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOPMTB
CXOPMTB	(Chandra X-ray sources in the Gum 31 nebula)
Write:	<<CXOPMTB JHHMMSS.ss+DDMMSS.s>>
N:	679
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	N=679 X-ray sources from Chandra X-ray observation of the Gum 31 nebula (in the Carina Nebula star forming complex).
Auth.:	Thomas Preibisch Universitaets-Sternwarte Muenchen
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOPS
CXOPS	(Chandra X-ray Observatory Plane Survey)
Write:	<<CXOPS JHHMMSS.s+DDMMSS>>
N:	about 10000
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Catalog of X-ray sources in the ChaMPlane multiwavelength survey. 2005ApJ...635..907H, 2006ApJS..163..160R: 2 first refs with CXOPS and ChOPS objects.
Notes:	ChaMPlane is a multiwavelength survey. This catalog (CXOPS) of X-ray sources will be joined by an optical catalog ChOPS. The two catalogs reference each other to provide X-ray and optical data, flux ratios etc for sources detected in both our Chandra and NOAO surveys. Infrared data will also be obtained and will follow the same convention, a separate IR catalog ChIPS with cross-referencing to the 2 others.
Notes:	The Chandra Multiwavelength Plane (ChaMPlane) Survey of the galactic plane incorporates serendipitous sources from selected Chandra pointings in or near the galactic plane (b < 12deg, >20 ksec, lack of bright diffuse or point sources) to measure or constrain the luminosity function of low-luminosity accretion sources in the Galaxy. The primary goal is to detect and identify accreting white dwarfs (cataclysmic variables, with space density still uncertain by a factor of >10-100), neutron stars and black holes (quiescent low mass X-ray binaries) to constrain their space densities and thus origin and evolution. Secondary objectives are to identify Be stars in high mass X-ray binaries and constrain their space densities, and to survey the H-R diagram for stellar coronal sources. A parallel optical imaging under the NOAO Long Term Survey program provides deep optical images using the Mosaic imager on the CTIO and KPNO 4-m telescopes. The 36x36arcmin optical images (Halpha, R, V and I) cover 5X the area of each enclosed Chandra ACIS FOV, providing an extended survey of emission line objects for comparison with Chandra. Spectroscopic followup of optical counterparts is then conducted, thus far with WIYN and Magellan. This catalog contains all ChaMPlane X-ray sources, their positions, properties and links to probable counterparts in our optical catalog. http://hea-www.harvard.edu/ChaMPlanebr 2005ApJ...635..907H: 1st ref. with CXOPS objects.
Ref:	=2005ApJ...635..907H
by	HONG J. , VAN DEN BERG M., SCHLEGEL E.M., GRINDLAY J.E., KOENIG X., LAYCOCK S., ZHAO P.
	Astrophys. J., 635, 907-919 (2005)
	X-ray processing of ChaMPlane fields: methods and initial results for selected anti-galactic center fields.
o	Table 8, col(1): <[ZGH2005] XSNNNNNBN-NNN> N=30 = Table 8, col(2): <CXOPS JHHMMSS.s+DDMMSS> N=30.
Ref:	=2006ApJS..163..160R
by	ROGEL A.B. , LUGGER P.M., COHN H.N., SLAVIN S.D., GRINDLAY J.E., ZHAO P., HONG J.
	Astrophys. J., Suppl. Ser., 163, 160-172 (2006)
	Three years of ChaMPlane northern field WIYN spectroscopy.
o	Tables 4 to 8: <ChOPS JHHMMSS.ss+DDMMSS.s> N=5+4+7+2+4. Tables 6 to 8: <CXOPS JHHMMSS.s+DDMMSS> N=7+5+26. Table 4: <[RLC2006] CVN> (Nos CV1-CV5), <[RLC2006] XBN> (Nos XB1, XB2).
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOPTM
CXOPTM	(Chandra X-ray Observatory, Pravdo+Tsuboi+Maeda)
Write:	<<CXOPTM JHHMMSS.s+DDMMSS>>
N:	94
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra X-ray Observatory-ACIS observation of the HH 80-81 region. 94 X-ray sources were detected including HH objects and pre-main-sequence stars.
Ref:	=2004ApJ...605..259P
by	PRAVDO S.H. , TSUBOI Y., MAEDA Y.
	Astrophys. J., 605, 259-271 (2004)
	X-rays from HH 80, HH 81, and the central region.
o	Table 1, col(1): format NN (Nos 1-94) is not used in SIMBAD.
o	Table 1: <CXOPTM JHHMMSS.s+DDMMSS> N=94.
=E=	Catalogue in electronic form as J/ApJ/605/259
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOPZ
CXOPZ	(Chandra X-ray Observatory, Preibisch+Zinnecker)
Write:	<<CXOPZ JHHMMSS.s+DDMMSS>> <<CXOPZ NNN>>
N:	215
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	X-ray sources detected in the Chandra/ACIS observation of IC 348.
in source:	IC 348
Ref:	=2001AJ....122..866P
by	PREIBISCH T. , ZINNECKER H.
	Astron. J., 122, 866-875 (2001)
	Deep Chandra X-ray observatory imaging study of the very young stellar cluster IC 348.
o	Objects 'X-NN' = '[PZH96] NN' in SIMBAD. 2MASS J034433+320131 not identified.
o	Table 1: <CXOPZ NNN> (Nos 1-215) = <CXOPZ JHHMMSS.s+DDMMSS> N=215.
=E=	Catalogue in electronic form as J/AJ/122/866
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXORRS
CXORRS	(Chandra X-ray Observatory, Ramirez+Rebull+Stauffer)
Write:	<<CXORRS JHHMMSS.s+DDMMSS>>
N:	263+417
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	X-ray sources detected with ACIS-I on board of the Chandra X-ray Observatory in a field of NGC2264 and two fields in Orion. See also [RRS2004]
in source:	NGC 2264
in source:	Orion = M 42 = NGC 1976
Ref:	=2004AJ....127.2659R
by	RAMIREZ S.V. , REBULL L., STAUFFER J., HEARTY T., HILLENBRAND L., JONES B., MAKIDON R., PRAVDO S., STROM S., WERNER M.
	Astron. J., 127, 2659-2673 (2004)
	Chandra X-ray observations of young clusters. I. NGC 2264 data.
o	Table 1, Col(1): <[RRS2004] NGC 2264 NNN> N=263 among (Nos 1-311) = Table 1, Col(2): <CXORRS JHHMMSS.s+DDMMSS> N=263.
Ref:	=2004AJ....128..787R
by	RAMIREZ S.V. , REBULL L., STAUFFER J., STROM S., HILLENBRAND L., HEARTY T., KOPAN E.L., PRAVDO S., MAKIDON R., JONES B.
	Astron. J., 128, 787-804 (2004)
	Chandra X-ray observations of young clusters. II. Orion flanking fields data.
o	In tables 4, 5: cross-id. HBJM NNNNN not in SIMBAD.
o	Table 1, Col(1): <[RRS2004] NOFF WNNN> N=203 among (Nos N001 to N256) = Table 1, Col(2): <CXORRS JHHMMSS.s+DDMMSS> N=203. Table 1, Col(1): <[RRS2004] SOFF WNNN> N=214 among (Nos S001 to S276) = Table 1, Col(2): <CXORRS JHHMMSS.s+DDMMSS> N=214.
=E=	Catalogue in electronic form as J/AJ/127/2659
=E=	Catalogue in electronic form as J/AJ/128/787
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOSEXSI
CXOSEXSI	(Chandra X-ray Observatory, Serendipitous Extragal. X-ray Source Identif.)
Write:	<<CXOSEXSI JHHMMSS.s+DDMMSS>>
N:	1034+877
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	SEXSI is a collaboration between researchers at Caltech and Columbia University to obtain a large sample of Serendipitous Extragalactic X-ray Source Identifications by extracting complete, hard (2.0-10.0keV) X-ray source lists from high Galactic latitude X-ray source lists from high Galactic latitude Chandra Observatory fields, and then to obtain photometric and spectroscopic identifications. 2003ApJ...596..944H, Table 4: source catalog, Table 6: soft-band-only source catalog. Optical imaging of the 1034 sources in 2005ApJS..156...35E
Ref:	=2003ApJ...596..944H
by	HARRISON F.A. , ECKART M.E., MAO P.H., HELFAND D.J., STERN D.
	Astrophys. J., 596, 944-956 (2003)
	The Serendipitous Extragalactic X-ray Source Identification program. I. Characteristics of the hard X-ray sample.
o	Tables 4, 6: <CXOSEXSI JHHMMSS.s+DDMMSS> N=1034+879.
=E=	Catalogue in electronic form as J/ApJ/596/944
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOSW
CXOSW	(Chandra X-ray Observatory, SWIRE)
Write:	<<CXOSW JHHMMSS.s+DDMMSS>>
N:	775
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Moderate-depth Chandra survey in the Lockman Hole Field of the Spitzer/SWIRE Legacy Survey.
Ref:	=2009ApJS..185..433W
by	WILKES B.J. , KILGARD R., KIM D.-W., KIM M., POLLETTA M., LONSDALE C., SMITH H.E., SURACE J., OWEN F.N., FRANCESCHINI A., SIANA B., SHUPE D.
	Astrophys. J., Suppl. Ser., 185, 433-450 (2009)
	The SWIRE/Chandra survey: the X-ray sources.
o	Tables 3-4, 7: <CXOSW JHHMMSS.s+DDMMSS> N=775.
=E=	Catalogue in electronic form as J/ApJS/185/433
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOTr16
CXOTr16	(Chandra X-ray Observatory, Trumpler 16)
Write:	<<CXOTr16 JHHMMSS.ss+DDMMSS.s>>
N:	1035
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS-I observations at the center of Cl Trumpler 16. See also [ADM2008].
in source:	Cl Trumpler 16
Ref:	=2008A&A...490.1055A
by	ALBACETE-COLOMBO J.F. , DAMIANI F., MICELA G., SCIORTINO S., HARNDEN F.R.Jr
	Astron. Astrophys., 490, 1055-1070 (2008)
	An X-ray survey of low-mass stars in Trumpler 16 with Chandra.
o	Table 1, col(2): the ID CXOCYG (ID for sources in the Association Cyg OB 2) is a misprint, we have created CXOTr16 for sources in Cl Trumpler 16.
o	Table 1, col(1): <[ADM2008] NNNN> (Nos 1-1035) = Table 1, col(2): <CXOTr16 JHHMMSS.ss+DDMMSS.s> N=1035.
=E=	Catalogue in electronic form as J/A+A/490/1055
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: CXOU
CXOU	(Chandra X-ray Observatory, Unregistered)= (CXU)
Write:	<<CXOU JHHMMSS.s+DDMMSS>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	CXOU, where U means "unregistered", may be used for the occasional sources found/published by individuals using Chandra X-ray Observatory data. See CXO.
Auth.:	ROTS A.+
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CXOUDS
CXOUDS	(Chandra X-ray Observatory UDS survey)
Write:	<<CXOUDS JHHMMSS.s+DDMMSS>>
N:	868
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Wide and deep Chandra observations of N=868 band-merged point sources in the Subaru-XMM Deep/UKIDSS Ultra Deep Survey (SXDS/UDS) field.
Ref:	=2018ApJS..236...48K
by	KOCEVSKI D.D. , HASINGER G., BRIGHTMAN M., NANDRA K., GEORGAKAKIS A., CAPPELLUTI N., CIVANO F., LI Y., LI Y., AIRD J., ALEXANDER D.M., ALMAINI O., BRUSA M., BUCHNER J., COMASTRI A., CONSELICE C.J., DICKINSON M.A., FINOGUENOV A., GILLI R., KOEKEMOER A.M., MIYAJI T., MULLANEY J.R., PAPOVICH C., ROSARIO D., SALVATO M., SILVERMAN J.D., SOMERVILLE R.S., UEDA Y.
	Astrophys. J., Suppl. Ser., 236, 48-48 (2018)
	X-UDS: the Chandra legacy survey of the UKIDSS Ultra Deep Survey field.
o	Table 4, col(2): <CXOUDS JHHMMSS.s+DDMMSS> N=868 = Table 4, col(1): <[KHB2018] xuds NNN> (Nos 001-868).
=E=	Catalogue in electronic form as <J/ApJS/236/48/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CXOUGC
CXOUGC	(Chandra X-ray Observatory Unregistered, Galactic Center)
*****	Avoid the usage of CXOUGC, prefer CXOGC
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOVVV
CXOVVV	(Chandra X-ray Observatory Vista Variables in Via Lactea probable cluster member)
Write:	<<CXOVVV JHHMMSS.ss+DDMMSS.s>>
N:	2148
Object:	* in Cl* (SIMBAD class: Star)
Note:	The CXOVVV catalog is a list of probable cluster members in NGC 6231 based on observations from the Chandra X-ray Observatory (CXO) and the Vista Variables in the Via Lactea (VVV) survey. This study provides a greatly expanded membership catalog based on a reanalysis of archival CXO observations using a methodology with improved sensitivity to faint X-ray sources and deeper catalogs of near-infrared counterparts. The tabulated probable cluster members range from OB stars to brown-dwarf candidates and from Class II to Class III pre-main-sequence stars. The CXOVVV catalog will be published in an electronic table (Table 3) in the following paper submitted to the Astronomical Journal: "The Structure of the Young Star Cluster NGC 6231. I. Stellar Population" by Michael A. Kuhn, Nicolas Medina, Konstantin V. Getman, Eric D. Feigelson, Mariusz Gromadzki, Jordanka Borissova, and Radostin Kurtev. A second paper entitled "The Structure of the Young Star Cluster NGC 6231. II. Structure, Formation, and Fate" is planned for submissing to the AAS Journals in May, 2017.
Notes:	The manuscript of Paper I and the CXOVVV catalog (FITS format) is available from the following URLs: https://drive.google.com/open?id=0B6YxlTWmOFVQQWZGejhBQVd2SG8 http://astro.psu.edu/mystix
Ref:	=2017AJ....154...87K
by	KUHN M.A. , MEDINA N., GETMAN K.V., FEIGELSON E.D., GROMADZKI M., BORISSOVA J., KURTEV R.
	Astron. J., 154, 87-87 (2017)
	The structure of the young star cluster NGC 6231. I. Stellar population.
o	Table 3: <CXOVVV JHHMMSS.ss+DDMMSS.s> N=2148. Universidad de Valpara?so
=E=	Catalogue in electronic form as <J/AJ/154/87/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOW3
CXOW3	(CXO, W 3 star forming region) >>>>>> New acronym being registered
Object:	(X)
Auth.:	DELGADO-MARTI H.J.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOW40
CXOW40	(CXO, W 40 star forming region)
Write:	<<CXOW40 JHHMMSS.ss+DDMMSS.s>>
N:	225
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS observations of the HII region W 40. See also [KGF2010].
in source:	W 40
Ref:	=2010ApJ...725.2485K
by	KUHN M.A. , GETMAN K.V., FEIGELSON E.D., REIPURTH B., RODNEY S.A., GARMIRE G.P.
	Astrophys. J., 725, 2485-2506 (2010)
	A Chandra observation of the obscured star-forming complex W40.
o	Tables 1, 2, 4: <[KGF2010] NNN> (Nos 1-225) = <CXOW40 JHHMMSS.ss+DDMMSS.s> N=225.
=E=	Catalogue in electronic form as <J/ApJ/725/2485/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CXOWSB
CXOWSB	(CXO, Wolk+Spitztbart+Bourke+) (Not yet in Simbad)
Write:	<<CXOWSB JHHMMSS.s+DDMMSS>>
N:	about 400
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	X-ray study of the star forming region RCW 108.
in source:	RCW 108
Auth.:	WOLK S.
=E=	Catalogue in electronic form as <J/AJ/135/693/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOXB
CXOXB	(CXO, XBootes)
Write:	<<CXOXB JHHMMSS.s+DDMMSS>>
N:	43+3293
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Large Area Chandra X-ray Survey of the Bootes field of the NOAO Deep Wide-Field Survey (NDWFS) called XBootes survey. The catalog is presented in paper I: 2005ApJS..161....1M
Ref:	=2005ApJS..161....9K
by	KENTER A. , MURRAY S.S., FORMAN W.R., JONES C., GREEN P., KOCHANEK C.S., VIKHLININ A., FABRICANT D., FAZIO G., BRAND K., BROWN M.J.I., DEY A., JANNUZI B.T., NAJITA J., McNAMARA B., SHIELDS J., RIEKE M.
	Astrophys. J., Suppl. Ser., 161, 9-20 (2005)
	XBootes: an X-ray survey of the NDWFS Bootes field. II. The X-ray source catalog.
o	Format first choosen by authors is CXOXB and not CXO XB as in this paper.
o	Tables 1, 3: <CXOXB JHHMMSS.s+DDMMSS> N=43+3293.
=E=	Catalogue in electronic form as J/ApJS/161/9
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXOYECDF
CXOYECDF	(CXO, Yale Extended CDFS source)
Write:	<<CXOYECDF JHHMMSS.s+DDMMSS>>
N:	651
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS observations of the Extended Chandra Deep Field South Survey. See also [VTU2006].
in source:	NAME ECDFS
Ref:	=2006AJ....131.2373V
by	VIRANI S.N. , TREISTER E., URRY C.M., GAWISER E.
	Astron. J., 131, 2373-2382 (2006)
	The Extended Chandra Deep Field-South survey: X-ray point-source catalog.
o	Tables 4, 5: <[VTU2006] NNN> (Nos 1-651) = <CXOYECDF JHHMMSS.s+DDMMSS> N=651. Table 6: <[VTU2006] Collapsed NN> (Nos 1-70).
=E=	Catalogue in electronic form as J/AJ/131/2373
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: CXR
CXR	(Cygnus X, Ridge)
Write:	<<CXR NN>>
N:	13
Object:	Ridge (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Table 6: (Nos 1-13), Ridges in Cygnus X
in source:	NAME Cyg X
Ref:	=1991A&A...241..551W
by	WENDKER H.J. , HIGGS L.A., LANDECKER T.L.
	Astron. Astrophys., 241, 551-580 (1991)
	The Cygnus X region. XVIII. A detailed investigation of radio-continuum structure on large and small scales.
o	Table 2: <18P NNNA> (Nos 1-103), N=109. Table 3: <19P NNA> (Nos 1-48), N=50. Table 4: <EXC6-NNA> (Nos 1-41), N=47. Table 6: <CXR NN> (Nos 1-13), N=13, Table 7: <CXH N> (Nos 1-6), N=6
=E=	Catalogue in electronic form as J/A+A/241/551
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: CXS
CXS	(COSMOS - X-band and S-band) (Not yet in Simbad)
*****	Avoid the usage of CXS, prefer COSMOS-XS
Origin	of the Acronym: L (2020ApJ...903..139A)
Details on Acronym: CXU
CXU	(Chandra X-ray, Unregistered)
Origin	of the Acronym: L (2003A	A.397.1011S)
Details on Acronym: [CY2004]
[CY2004]	(Chen+Yao, 2004)= (NIRS)
Write:	<<[CY2004] NIRS NN>> <<[CY2004] H2 N>>
N:	39+8
Object:	(IR) + H2 (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	NIR observations at the 1.88m telescope at Okayama Astronomical Observatory. N=39 NIR point sources in the nebular region, and N=8 H2 emission peaks in IRAS 23151+5912.
in source:	IRAS 23151+5912
Ref:	=2004ChJAA...4..284C
by	CHEN X.-P. , YAO Y.-Q.
	Chinese J. Astron. Astrophys., 4, 284-298 (2004)
	Near-infrared observations of the massive star forming region IRAS 23151+5912.
o	Table 1: <[CY2004] NIRS NN> (Nos 1-39). Table 2: <[CY2004] H2 N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: cya
cya	(Cygnus, field A)
*****	Avoid the usage of cya, prefer [ABC90]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: cyb
cyb	(Cygnus, field B)
*****	Avoid the usage of cyb, prefer [ABC90]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: cyc
cyc	(Cygnus, field C)
*****	Avoid the usage of cyc, prefer [ABC90]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CYD2005]
[CYD2005]	(Carney+Yong+De Almeida+, 2005)
Write:	<<[CYD2005] NNNNN>>
N:	8472
Object:	* (SIMBAD class: Star)
Note:	BVI photometry at the CTIO Curtis Schmidt telescope. Spectroscopic observations at the CTIO 4m Blanco telescope. Search for red giants in the direction of the southern warp of the galactic disk.
Ref:	=2005AJ....130.1111C
by	CARNEY B.W. , YONG D., DE ALMEIDA M.L.T., SEITZER P.
	Astron. J., 130, 1111-1126 (2005)
	Elemental abundance ratios in stars of the outer galactic disk. II. Field red giants.
o	Tables 2, 3: <[CYD2005] NNNNN> N=8472 among (Nos 95-11802).
=E=	Catalogue in electronic form as J/AJ/130/1111
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Cyg
Cyg	(Cygnus)
*****	Avoid the usage of Cyg, prefer Glazar
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Cyg
Cyg
*****	Avoid the usage of Cyg, prefer [MWC53]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Cyg
Cyg	(Cygnus)
*****	Avoid the usage of Cyg, prefer Vulcan
Origin	of the Acronym: L (2002ApJ...564..495J)
Details on Acronym: Cyg OB 2-
Cyg OB 2-	(Cyg OB2)
*****	Avoid the usage of Cyg OB 2-, prefer [MM53]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: CygX
CygX	(Cygnus X)
*****	Avoid the usage of CygX, prefer [MBS2007c]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CYM2001]
[CYM2001]	(Carlberg+Yee+Morris+, 2001)
Write:	<<[CYM2001] HHMMSS.s+DDMMSS>>
N:	190
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	N=190 galaxy groups in the CNOC2 survey.
Ref:	=2001ApJ...552..427C
by	CARLBERG R.G. , YEE H.K.C., MORRIS S.L., LIN H., HALL P.B., PATTON D.R., SAWICKI M., SHEPHERD C.W.
	Astrophys. J., 552, 427-444 (2001)
	Galaxy groups at intermediate redshift.
o	Coordinates in Table 1 are 1950 coordinates, not 2000.
o	Table 1: <[CYM2001] HHMMSS.s+DDMMSS> N=190.
=E=	Catalogue in electronic form as J/ApJ/552/427
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CYO2022]
[CYO2022]	(Chun+Yoon+Oh+, 2022)
Write:	<<[CYO2022] starNN>>
N:	14
Object:	Red Supergiant (SIMBAD class: RedSG = Red Supergiant)
Stat:	is completely incorporated in Simbad
Note:	MMT MMIRS spectroscopy of N=14 red supegiants in IC 1613.
in source:	IC 1613
Ref:	=2022ApJ...939...28C
by	CHUN S.-H. , YOON S.-C., OH H., PARK B.-G., HWANG N.
	Astrophys. J., 939, 28 (2022)
	Red Supergiant Stars in IC 1613 and Metallicity-dependent Mixing Length in the Evolutionary Model.
o	Table 2: <[CYO2022] starNN> (Nos star1-star14).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [CYT98]
[CYT98]	(Condon+Yin+Thuan+, 1998)
Write:	<<[CYT98] HHMMSS.s+DDMMSS>> <<[CYT98] HHMMSS.ss+DDMMSS.s>>
N:	14+2
Object:	G + * (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ROSAT/IRAS sample. N=14 galaxies which are not IRAS and RX sources + N=2 faint stars.
Ref:	=1998AJ....116.2682C
by	CONDON J.J. , YIN Q.F., THUAN T.X., BOLLER T.
	Astron. J., 116, 2682-2716 (1998)
	The ROSAT/IRAS galaxy sample revisited.
o	<[CYT98] HHMMSS.s+DDMMSS>, <[CYT98] HHMMSS.ss+DDMMSS.s>, N=14+2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CYW99]
[CYW99]	(Campos+Yahil+Windhorst+, 1999)
Write:	<<[CYW99] QN>> <<[CYW99] GN>>
N:	3+2
Object:	QSO + G (SIMBAD class: EmObj = Emission Object)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=3 QSO and N=2 Galaxies. Map in Fig.1
Ref:	=1999ApJ...511L...1C
by	CAMPOS A. , YAHIL A., WINDHORST R.A., RICHARDS E.A., PASCARELLE S., IMPEY C., PETRY C.
	Astrophys. J., 511, 1-4 (1999)
	A cluster or filament of galaxies at redshift z = 2.5?.
o	Table 1: <[CYW99] QN> (Nos Q1-Q3), <[CYW99] GN> (Nos G1-G2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CYY2004]
[CYY2004]	(Chen+Yao+Yang+, 2004) (Not yet in Simbad)
Write:	<<[CYY2004] DES-S87E>> <<[CYY2004] Knot A>> <<[CYY2004] AA N>>
N:	1+5+5
Object:	(Near IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	The polarimetric and spectroscopic study of Sh 2-87 reveal a Deeply Embedded Source (DES-S87E), 5 knots (Nos A-E) and 5 new sources (NS 1 to NS 5). See also [CZY2003].
in source:	SH 2-87
Ref:	=2004A&A...428..523C
by	CHEN X. , YAO Y., YANG J., JIANG Z., ISHII M.
	Astron. Astrophys., 428, 523-533 (2004)
	Near-infrared polarimetric and spectrometric study of the massive star-forming region S87.
o	Table 1: <[CYY2004] DES-S87E> N=1, <[CYY2004] Knot A> (Nos A-E). Fig.2, Table 2: <[CYY2004] AA N> (Nos NS 1 to NS 5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CYY2005]
[CYY2005]	(Chen+Yo+Yang+, 2005)= (NIRS)
Write:	<<[CYY2005] NIRS NNN>>
N:	164
Object:	(Near IR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	NIR observations at the Okayama Astronomical Observatory 1.88m telescope of the region around AFGL 5142.
in source:	RAFGL 5142
Ref:	=2005ApJ...629..288C
by	CHEN Y. , YAO Y., YANG J., ZENG Q., SATO S.
	Astrophys. J., 629, 288-298 (2005)
	Near-infrared imaging of the star formation region AFGL 5142.
o	Table 2: <[CYY2005] NIRS NNN> (Nos 1-164). Table 3: <[HTT95] Knot AN> (Nos G-Z, Y1) added.
=E=	Catalogue in electronic form as J/ApJ/629/288
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CYY2009]
[CYY2009]	(Chen+Yao+Yang+, 2009)
Write:	<<[CYY2009] Sh 2-NNN NIRS NNN>> <<[CYY2009] Sh 2-NNN ANN>>
N:	369+405+21+11
Object:	(NIR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	Okayama Astronomical Observatory 1.88m telescope OASIS NIR photometry of the HII regions Sh2-157 and Sh2-152.
in source:	SH 2-152
in source:	SH 2-157
Ref:	=2009ApJ...693..430C
by	CHEN Y. , YAO Y., YANG J., ZENG Q., SATO S.
	Astrophys. J., 693, 430-446 (2009)
	Near-infrared imaging of the star-forming regions Sh2-157 and Sh2-152.
o	Table 1: <[CYY2009] Sh 2-152 NIRS NNN> (Nos 1-369). Table 3: <[CYY2009] Sh 2-157 NIRS NNN> (Nos 1-405). Table 2: <[CYY2009] Sh 2-152 ANN> (Nos A1-A2, F1-F10, K1-K9). Table 4: <[CYY2009] Sh 2-152 ANN> (Nos A1-A2, F1-F7, K1-K2).
=E=	Catalogue in electronic form as <J/ApJ/693/430/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CYY99]
[CYY99]	(Chen+Yao+Yang+, 1999)= (NIRS)
Write:	<<[CYY99] NIRS NNN>> <<[CYY99] H2 NNa>>
N:	170+25
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	N=170 NIRS sources in the field of AFGL 5157. N=17 H2 emission knots, some knots have components 'NNa'.
Ref:	=1999AJ....117..446C
by	CHEN Y. , YAO Y., YANG J., HIRAO T., ISHII M., NAGATA T., SATO S.
	Astron. J., 117, 446-455 (1999)
	Near-infrared imaging of the star-forming region AFGL 5157.
o	Table 1: <[CYY99] NIRS NNN> (Nos 1-170). Table 2: <[CYY99] H2 NN> (Nos 1-12).
Ref:	=2003A&A...405..655C
by	CHEN Y. , YAO Y., YANG J., ZENG Q., SATO S.
	Astron. Astrophys., 405, 655-661 (2003)
	New detection of near-infrared H_{2} line emission in AFGL 5157.
o	Table 1: <[CYY99] H2 NNa> (Nos 3a, 13a-13b, 14-15, 16a-16g, 17) added.
=E=	Catalogue in electronic form as J/AJ/117/446
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CYZ2007]
[CYZ2007]	(Chen+Yang+Zhang, 2007)
Write:	<<[CYZ2007] NNN>>
N:	113
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Note:	IRAS, ISO, and 2MASS photometry of 113 J-type carbon stars from the literature.
Ref:	=2007AJ....134..214C
by	CHEN P.-S. , YANG X.-H., ZHANG P.
	Astron. J., 134, 214-222 (2007)
	Infrared study of J-type carbon stars based on Infrared Astronomical Satellite, Two Micron All Sky Survey, and Infrared Space Observatory data.
o	Table 1: <[CYZ2007] NNN> (Nos 1-113).
=E=	Catalogue in electronic form as J/AJ/134/214
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Cz
Cz	(Czernik)
*****	Avoid the usage of Cz, prefer Czernik
Details on Acronym: CZ
CZ	(Cape Zone)
*****	Avoid the usage of CZ, prefer CPC
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Cz01
Cz01	(Czoske+, 2001)
*****	Avoid the usage of Cz01, prefer [CKS2001]
Origin	of the Acronym: L (2006ApJ...643..764M)
Details on Acronym: [CZ2003]
[CZ2003]	(Christlein+Zabludoff, 2003)
Write:	<<[CZ2003] NNNNA-NNNNA NNN>> <<[CZ2003] SERA-NNNN NNN>>
N:	641+698+341+631+505+404
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Las Campanas observations. Galaxy Luminosity Functions of galaxies in 6 nearby clusters.
in source:	ACO 1060
in source:	ACO 1631
in source:	ACO 496
in source:	ACO 754
in source:	ACO 85
in source:	ACO 3266 = Ser 40-6
Ref:	=2003ApJ...591..764C
by	CHRISTLEIN D. , ZABLUDOFF A.I.
	Astrophys. J., 591, 764-783 (2003)
	Galaxy luminosity functions from deep spectroscopic samples of rich clusters.
o	Table 2: <[CZ2003] 1060A-NNNA NNN> N=641, <[CZ2003] 1631A-NNN NNN> N=698, <[CZ2003] 496A-NNNN NNN> N=341, <[CZ2003] 754A-NNNN NNN> N=631, <[CZ2003] 85A-NNNN NNN> N=505, <[CZ2003] SERA-NNNN NNN> N=404.
=E=	Catalogue in electronic form as J/ApJ/591/764
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CZB2020]
[CZB2020]	(Chen+Zahedy+Boettcher+, 2020)
Write:	<<[CZB2020] JHHMMSS.ss+DDMMSS.ss>>
N:	15
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=15 galaxies around Lyman limit systems (LLSs) of four QSO sightlines, as part of the Cosmic Ultraviolet Baryon Survey (CUBS).
Ref:	=2020MNRAS.497..498C
by	CHEN H.-W. , ZAHEDY F.S., BOETTCHER E., COOPER T.M., JOHNSON S.D., RUDIE G.C., CHEN M.C., WALTH G.L., CANTALUPO S., COOKSEY K.L., FAUCHER-GIGUERE C.-A., GREENE J.E., LOPEZ S., MULCHAEY J.S., PENTON S.V., PETITJEAN P., PUTMAN M.E., RAFELSKI M., RAUCH M., SCHAYE J., SIMCOE R.A., WEINER B.J.
	Mon. Not. R. Astron. Soc., 497, 498-520 (2020)
	The Cosmic Ultraviolet Baryon Survey (CUBS) - I. Overview and the diverse environments of Lyman limit systems at z < 1.
o	Table 7: <[CZB2020] JHHMMSS.ss+DDMMSS.ss> N=15.
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: CZC
CZC	(Cape Zone Catalog)
*****	Avoid the usage of CZC, prefer CPC
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [CZC2013]
[CZC2013]	(Coe+Zitrin+Carrasco+, 2013)
Write:	<<[CZC2013] MACS0647-JD>> <<[CZC2013] MACS0647-JDN>> <<[CZC2013] Na>>
N:	1+3+24
Object:	Grav. lensed image of a G + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Search for lensed galaxies in HST WFPC3/IR and ACS observations of MCS J0647.7+7015.
in source:	MCS J0647.0+7015
Ref:	=2013ApJ...762...32C
by	COE D. , ZITRIN A., CARRASCO M., SHU X., ZHENG W., POSTMAN M., BRADLEY L., KOEKEMOER A., BOUWENS R., BROADHURST T., MONNA A., HOST O., MOUSTAKAS L.A., FORD H., MOUSTAKAS J., VAN DER WEL A., DONAHUE M., RODNEY S.A., BENITEZ N., JOUVEL S., SEITZ S., KELSON D.D., ROSATI P.
	Astrophys. J., 762, 32 (2013)
	CLASH: three strongly lensed images of a candidate z ~ 11 galaxy.
o	Texte: <[CZC2013] MACS0647-JD> N=1, Table 3: <[CZC2013] MACS0647-JDN> (Nos JD1-JD3), Table 6: <[CZC2013] Na> N=24 (Nos 1a-9c)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Czernic
Czernic	(Czernik)
*****	Avoid the usage of Czernic, prefer Czernik
Details on Acronym: Czernik
Czernik	(Czernik)= (Cz) = (Czernic)
Write:	<<Cl Czernik NN>>
N:	45
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Ref:	=1966AcA....16...93C
by	CZERNIK M.
	Acta Astron., 16, 93-94 (1966)
	New open star clusters.
o	Table 1: <Cl Czernik NN> (Nos 1-45).
Details on Acronym: CzeV
CzeV	(Czech Variable)
Write:	<<CzeV NNNN>> <<CzeV NNNN CCC>>
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Catalogue of Czech variable stars (variables discovered in Czech Republic and/or by Czech observers). The on-line catalogue is available at http://var2.astro.cz/czev.php?lang=en
Ref:	=2006OEJV...23...55B
by	BRAT L.
	OEJV, 23, 55 (2006)
	The CzeV Catalogue - Czech Variable Stars.
o	<CzeV NNN>.
Ref:	=2017OEJV..185....1S
by	SKARKA M. , MASEK M., BRAT L., CAGAS P., JURYSEK J., HONKOVA K., ZEJDA M., SMELCER L., JELINEK M., LOMOZ F., TYLSAR M., TRNKA J., PEJCHA O., PINTR P., LEHKY M., JANIK J., CERVINKA L., PRIBIK V., MOTL D., WALTER F., ZASCHE P., KOSS K., HAJEK P., BILEK F., LISKA J., KUCAKOVA H., BODNAR F., BERANEK J., SAFAR J., MOUDRA M., ORSULAK M., PINTR M., SOBOTKA P., DREVENY R., JURANOVA A., POLAK J., POLSTER J., ONDERKOVA K., SMOLKA M., AUER R.F., KOCIAN R., HLADIK B., CAGAS P., GRES A., MULLER D., CAPKOVA H., KYSELY J., HORNOCH K., TRUPAROVA K., TIMKO L., BROZ M., BILEK M., SEBELA P., HANZL D., ZAMPACHOVA E., SECKA J., PRAVEC P., MRNAK P., SVOBODA P., EHRENBERGER R., NOVOTNY F., PODDANY S., PRUDIL Z., KUCHTAK B., STEGNER D.
	OEJV, 185, 1 (2017)
	CzeV - The Czech Variable Star Catalogue.
o	Table 4: <CzeV NNNN> (Nos 1-1228).
=E=	Catalogue in electronic form as <J/other/OEJV/185/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [CZG2014]
[CZG2014]	(Ciardullo+Zeimann+Gronwall+, 2014)
Write:	<<[CZG2014] JHHMMSS.ss+DDMMSS.s>>
N:	87
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=87 galaxies with Lyα and Hβ emission lines in the COSMOS, GOODS-North and -South fields. Use of HST WFC3 data.
in source:	NAME COSMOS Field
in source:	NAME GOODS North Field
in source:	NAME GOODS South Field
Ref:	=2014ApJ...796...64C
by	CIARDULLO R. , ZEIMANN G.R., GRONWALL C., GEBHARDT H., SCHNEIDER D.P., HAGEN A., MALZ A.I., BLANC G.A., HILL G.J., DRORY N., GAWISER E.
	Astrophys. J., 796, 64 (2014)
	Hubble Space Telescope emission line galaxies at z ~ 2: the Lyα escape fraction.
o	Table 1: <[CZG2014] JHHMMSS.ss+DDMMSS.s> N=87.
=E=	Catalogue in electronic form as J/ApJ/796/64
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CZH2003]
[CZH2003]	(Ciliegi+Zamorani+Hasinger+, 2003)= (LOCK-6cm)
Write:	<<[CZH2003] LOCK-6cm JHHMMSS+DDMMSSA>>
N:	70
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Deep VLA radio image at 6cm of the Lockman Hole. N=63 radio-sources, among which 2 have multiple components 'A' and have been treated as a single radio-source (format ending with 'T').
in source:	NAME Lockman Hole
Ref:	=2003A&A...398..901C
by	CILIEGI P. , ZAMORANI G., HASINGER G., LEHMANN I., SZOKOLY G., WILSON G.
	Astron. Astrophys., 398, 901-918 (2003)
	A deep VLA survey at 6 cm in the Lockman Hole.
o	Table 1: <[CZH2003] LOCK-6cm JHHMMSS+DDMMSSA> N=70.
=E=	Catalogue in electronic form as J/A+A/398/901
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CZM2007]
[CZM2007]	(Carraro+Zinn+Moni Bidin, 2007)
Write:	<<[CZM2007] NNNN>>
N:	952
Object:	*inCl (SIMBAD class: Star)
Note:	VLT deep CCD photometry of the globular cluster Whiting 1.
in source:	NAME WHITING 1
Ref:	=2007A&A...466..181C
by	CARRARO G. , ZINN R., MONI BIDIN C.
	Astron. Astrophys., 466, 181-189 (2007)
	Whiting 1: the youngest globular cluster associated with the Sagittarius dwarf spheroidal galaxy.
o	Catalog: <[CZM2007] NNNN> N=952 among (Nos 1-1649).
=E=	Catalogue in electronic form as J/A+A/466/181
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CZY2003]
[CZY2003]	(Chen+Zheng+Yao+, 2003)= (NIRS)
Write:	<<[CZY2003] S87W>> <<[CZY2003] S87E NIRS NNN>> <<[CZY2003] H2 region AN>> <<[CZY2003] S87W NIRS A>>
N:	2+21+6+2
Object:	(Near IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Near IR images of Sh 2-87 reveal 2 bright nebula, and NIRS peaks in each of these. See also [CYY2004].
in source:	SH 2-87
Ref:	=2003A&A...401..185C
by	CHEN Y. , ZHENG X.-W., YAO Y., YANG J., SATO S.
	Astron. Astrophys., 401, 185-192 (2003)
	Near-infrared imaging of the star forming region S87.
o	Fig.1, text: <[CZY2003] S87W> (Nos S87E, S87W). Fig.2, Table 1: <[CZY2003] S87E NIRS NNN> N=21 among 111. Fig.6: <[CZY2003] H2 region AN> (Nos A-E, B2). Fig.7: <[CZY2003] S87W NIRS A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CZZ2013]
[CZZ2013]	(Cepas+Zdanavicius+Zdanavicius+, 2013)= ([CZZ2013a]) (Not yet in Simbad)
Write:	<<[CZZ2013] NNN>>
N:	922
Object:	* (SIMBAD class: Star)
Note:	Vilnius photometry for N=922 down to V∼17mag in a 1.5 sq. deg. field at the northern edge of the HII region Sh 2-205, obtained with the Matsukov 35-51cm telescope of the Moletai Observatory (Lithuania).
in source:	SH 2-205
Ref:	=2013BaltA..22..223C
by	CEPAS V. , ZDANAVICIUS J., ZDANAVICIUS K., STRAIZYS V., LAUGALYS V.
	BaltA, 22, 223-242 (2013)
	Seven-color photometry and classification of stars in the vicinity of the emission nebula Sh2-205.
o	Table 3: <[CZZ2013] NNN> (Nos 1-922).
=E=	Catalogue in electronic form as <J/BaltA/22/223/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CZZ2013a]
[CZZ2013a]	(Cepas+Zdanavicius+Zdanavicius+, 2013) (Not yet in Simbad)
*****	Avoid the usage of [CZZ2013a], prefer [CZZ2013]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CZZ2013b]
[CZZ2013b]	(Cepas+Zdanavicius+Zdanavicius+, 2013) (Not yet in Simbad)
Write:	<<[CZZ2013b] NNN>>
N:	727
Object:	* (SIMBAD class: Star)
Note:	Vilnius photometry for N=727 stars down to V∼17 mag in a 1.5 squ. deg. field in the region of dark cloud TGU H994 P1 in Camelopardalis, obtained with the Matsukov 35-51cm telescope of the Moletai Observatory (Lithuania).
in source:	TGU H994: TGU H994 P1 = TGU H994 P1
Ref:	=2013BaltA..22..243C
by	CEPAS V. , ZDANAVICIUS J., ZDANAVICIUS K., STRAIZYS V., LAUGALYS V.
	BaltA, 22, 243-258 (2013)
	Seven-color photometry and classification of stars in the vicinity of the dark cloud TGU H994 (LDN 1399, 1400 and 1402).
o	Table 3: <[CZZ2013b] NNN> (Nos 1-727).
=E=	Catalogue in electronic form as <J/BaltA/22/243/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [CZZ2016]
[CZZ2016]	(Chen+Zhang+Zhang+, 2016)
Write:	<<[CZZ2016] IRS N>>
N:	4
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	SAAO IRSF 1.4m telescope SIRPOL and Spitzer IRAC photometric observations of N=4 young stellar objects (YSOs) in the star-forming clump N4W. Use of archival UKIDSS GPS DR6 data.
in source:	[CPA2006] N4
Ref:	=2016ApJ...822..114C
by	CHEN Z. , ZHANG S., ZHANG M., JIANG Z., TAMURA M., KWON J.
	Astrophys. J., 822, 114-114 (2016)
	Coeval intermediate-mass star formation in N4W.
o	SMM1 is AGAL G011.812+00.837 in SIMBAD. N4W is not in SIMBAD (no coordinates).
o	Table 1: <[CZZ2016] IRS N> (Nos IRS 1-IRS 4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: D
D	(Drake) (Not yet in Simbad)
*****	Avoid the usage of D, prefer [D59]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: D
D	(Dominion astroph. obs.)
*****	Avoid the usage of D, prefer [CCS85]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: D
D	(Dolidze)
*****	Avoid the usage of D, prefer [D75b]
Origin	of the Acronym: L (1999A&AS..134..255K)
Details on Acronym: D
D	(Dressler)
*****	Avoid the usage of D, prefer [D81]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: D
D	(Dachs)
*****	Avoid the usage of D, prefer Dachs
Origin	of the Acronym: L = Found in the literature
Details on Acronym: D
D	(D'Odorico+)
*****	Avoid the usage of D, prefer DBS
Origin	of the Acronym: L (1980A&AS...40...67D)
Details on Acronym: D
D	(Davis)
*****	Avoid the usage of D, prefer [DGW65]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: D
D	(Dufour+)
*****	Avoid the usage of D, prefer [DTJ80]
Origin	of the Acronym: L (1999ApJ...510..104B)
Details on Acronym: D
D	(Donahue+)
*****	Avoid the usage of D, prefer [DVG98]
Origin	of the Acronym: L (1999ApJ...522...39T)
Details on Acronym: D
D	(Donahue+)
*****	Avoid the usage of D, prefer [DVG98]
Origin	of the Acronym: L (1999ApJ...522...39T)
Details on Acronym: D
D	(cloud complex labelled D)
*****	Avoid the usage of D, prefer [H68]
Details on Acronym: 3D-HST
3D-HST	(3D-HST)
*****	Avoid the usage of 3D-HST, prefer [SWM2014]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: D06
D06	(De Buizer, 2006) (Not yet in Simbad)
Write:	<<D06 N>>
N:	5
Object:	(Mid IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Mid-IR structure of IRAS 20126+4104.
in source:	IRAS 20126+4104
Ref:	=2007ApJ...654L.147D
by	DE BUIZER J.M.
	Astrophys. J., 654L, 147-150 (2007)
	The complex mid-infrared structure at the heart of IRAS 20126+4104.
o	Fig.1: <D06 N> (Nos 1-5).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: D0K
D0K	(Deep 0 hour field)
Write:	<<D0K NNN>>
Object:	G (SIMBAD class: Galaxy)
Note:	The survey was first described in 1996ApJ...462L...9C.
Ref:	=1999ApJ...512...30C
by	COHEN J.G. , BLANDFORD R., HOGG D.W., PAHRE M.A., SHOPBELL P.L.
	Astrophys. J., 512, 30-47 (1999)
	Caltech faint galaxy redshift survey. VIII. Analysis of the field J0053+1234.
o	Table 1: <D0K NNN> N=139.
Ref:	=1999ApJS..120..171C
by	COHEN J.G. , HOGG D.W., PAHRE M.A., BLANDFORD R., SHOPBELL P.L., RICHBERG K.
	Astrophys. J., Suppl. Ser., 120, 171-178 (1999)
	Caltech faint galaxy redshift survey. VII. Data analysis techniques and redshifts in the field J0053+1234.
o	Table 3: <D0K NNN> (Nos 1-189) and N=13 among (Nos 450-984).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [D2003]
[D2003]	(Dahlen, 2003)= ([D2003a])
Write:	<<[D2003] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations. Nearest G of SN 2002KL.
Ref:	=2003IAUC.8083....1D
by	DAHLEN T.
	IAU Circ., 8083, 1-None (2003)
	Supernova 2002kl.
o	<[D2003] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2003a]
[D2003a]	(Dahlen, 2003)
*****	Avoid the usage of [D2003a], prefer [D2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2003b]
[D2003b]	(Doi, 2003)
Write:	<<[D2003b] JHHMMSS.ss+DDMMSS.s>>
N:	5
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Subaru observations. Host galaxies of SN 2002KZ, SN 2002LA, SN 2002LB, SN 2002LC, and SN 2002LD.
Ref:	=2003IAUC.8121....3D
by	DOI M.
	IAU Circ., 8121, 3-None (2003)
	Supernovae 2002kz, 2002la, 2002lb, 2002lc, 2002ld.
o	<[D2003b] JHHMMSS.ss+DDMMSS.s> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2004]
[D2004]	(Davidge, 2004)
Write:	<<[D2004] NN>>
N:	33
Object:	* + Cluster of * (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	CFHTIR camera on the CFHT. Observations of NGC 3077.
in source:	NGC 3077
Ref:	=2004AJ....127.1460D
by	DAVIDGE T.J.
	Astron. J., 127, 1460-1471 (2004)
	Stars, star clusters, and dust in NGC 3077.
o	Table 1: <[D2004] NN> (Nos 1-33).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2005]
[D2005]	(Dahlem, 2005)= ([D2005a])
Write:	<<[D2005] N>>
N:	5
Object:	Feature (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA HI study of the Grus Quartet reveals spectacular tidal structures: 1: weak tidal features on opposite sides of NGC 7552. 2: a dwarf galaxy: LCRS B231454.2-423320 3: an HI gas cloud west of NGC 7582. 4: an HI nonthermal tail from NGC 7582. 5: a faint tidal tail south end of NGC 7582.
in source:	NAME Grus Quartet
Ref:	=2005A&A...429L...5D
by	DAHLEM M.
	Astron. Astrophys., 429, 5-8 (2005)
	Intergalactic neutral hydrogen gas in the Grus quartet of galaxies.
o	Figs 1, 2: <[D2005] N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2005a]
[D2005a]	(Dahlem, 2005)
*****	Avoid the usage of [D2005a], prefer [D2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2005b]
[D2005b]	(Davidge, 2005) (Not yet in Simbad)
Write:	<<[D2005b] Cluster N>>
N:	2
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Gemini South and CFH telescopes are use to study NGC 55. 2 stellar clusters are found.
in source:	NGC 55
Ref:	=2005ApJ...622..279D
by	DAVIDGE T.J.
	Astrophys. J., 622, 279-293 (2005)
	The disk and extraplanar regions of NGC 55.
o	Fig.2, text: <[D2005b] Cluster N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2005c]
[D2005c]	(Drake, 2005)= (DC) = (DGC)
Write:	<<[D2005c] DCN>> <<[D2005c] DGCN>>
Object:	Cluster of * + Cluster of G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Systematic search for the USNO-A2.0 catalogue for stellar cluster candidates which may have been missed in previous searches. 8 new stellar clusters are found, designated as 'DC1' to 'DC8', and 3 candidate galaxy clusters designated as 'DGC1' to 'DGC3'.
Ref:	=2005A&A...435..545D
by	DRAKE A.J.
	Astron. Astrophys., 435, 545-550 (2005)
	Cluster candidates from the USNO-A2.0 catalogue.
o	Table 1: <[D2005c] DCN> (Nos DC1 to DC8), <[D2005c] DGCN> (Nos DGC1 to DGC3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2005d]
[D2005d]	(Durant, 2005)
Write:	<<[D2005d] A>>
N:	10
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	NIR observations with the Magellan Clay telescope Stars within or near the Chandra error circle of 1E 1841-04.5.
Ref:	=2005ApJ...632..563D
by	DURANT M.
	Astrophys. J., 632, 563-566 (2005)
	A deep infrared search for AXP 1E 1841-045.
o	Fig.1, Table 1: <[D2005d] A> (Nos A-J).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2006]
[D2006]	(Davies, 2006)= ([D2006a])
Write:	<<[D2006] LCANN>>
N:	79
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	N=79 new variable stars.
Ref:	=2006JAVSO..34..222D
by	DAVIES D.
	JAVSO, 34, 222-230 (2006)
	New Northern Hemisphere Variables.
o	Table 1: <[D2006] LCDNN>, <[D2006] LCENN>, <[D2006] LCFNN>, <[D2006] LCGNN>, N=79.
=E=	Catalogue in electronic form as J/other/JAVSO/34.222
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2006a]
[D2006a]	(Davies, 2006)
*****	Avoid the usage of [D2006a], prefer [D2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2006b]
[D2006b]	(De Buizer, 2006) (Not yet in Simbad)
Write:	<<[D2006b] NN>>
N:	10
Object:	(Mid IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Mid IR sources at 11.7mu.m in the region of GAL 035.2-00.74.
Ref:	=2006ApJ...642L..57D
by	DE BUIZER J.M.
	Astrophys. J., 642, 57-60 (2006)
	The remarkable mid-infrared jet of the massive young stellar object G35.20-0.74.
o	Fig.1: <[D2006b] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2007]
[D2007]	(Davidge, 2007)
Write:	<<[D2007] JHHMMSS.s+DDMMSS.s>>
N:	6
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Stat:	is completely incorporated in Simbad
Note:	CFHT WIRCam and MegaCam observations of NGC 2403.
in source:	NGC 2403
Ref:	=2007ApJ...664..820D
by	DAVIDGE T.J.
	Astrophys. J., 664, 820-839 (2007)
	The disk and extraplanar regions of NGC 2403.
o	Table 2: <[D2007] JHHMMSS.s+DDMMSS.s> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2008]
[D2008]	(Davidge, 2008)= ([D2008a])
Write:	<<[D2008] N>>
N:	5
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	CFHT MegaCam and WIRCam observations of M 82.
in source:	M 82 = NGC 3034
Ref:	=2008AJ....136.2502D
by	DAVIDGE T.J.
	Astron. J., 136, 2502-2521 (2008)
	And the rest: the stellar archeological record of M82 outside the central starburst.
o	Table 1: <[D2008] N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2008a]
[D2008a]	(Davidge, 2008)
*****	Avoid the usage of [D2008a], prefer [D2008]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2008b]
[D2008b]	(Davidge, 2008)= (TDO)
Write:	<<[D2008b] TDO N>>
N:	3
Object:	Tidal debris (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	CFHT MegaCam observations of the debris field around M81.
in source:	M 81
Ref:	=2008PASP..120.1145D
by	DAVIDGE T.J.
	PASP, 120, 1145-1160 (2008)
	The identification of new stellar groupings in the M81 debris field.
o	Fig.1, Table 1: <[D2008b] TDO N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2012]
[D2012]	(Da Costa, 2012)
Write:	<<[D2012] NNNNNN>>
N:	34
Object:	* (SIMBAD class: Star)
Note:	AAT AAOmega observations of the ome Cen Cluster. See also [DC2008].
in source:	ome Cen = NGC 5139
Ref:	=2012ApJ...751....6D
by	DA COSTA G.S.
	Astrophys. J., 751, 6 (2012)
	The dynamics of the outer parts of ω Centauri.
o	Tables 1-2: <[DC2008] NN-N-NNNNN> N=24 added, <[D2012] NNNNNN> N=34 among (Nos 44610-210569).
=E=	Catalogue in electronic form as J/ApJ/751/6
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2013]
[D2013]	(Dawson, 2013)
Write:	<<[D2013] JHHMMSS.sss+DDMMSS.ss>>
N:	708
Object:	G (SIMBAD class: Galaxy)
Note:	N=708 galaxies in the Musket Bullet Cluster redshift catalog.
in source:	NAME Musket Ball Cluster = DLSCL J09162+2951
Ref:	=2013ApJ...772..131D
by	DAWSON W.A.
	Astrophys. J., 772, 131 (2013)
	The dynamics of merging clusters: a Monte Carlo solution applied to the Bullet and Musket Ball Clusters.
o	<NAME Musket Ball Cluster> N=1. Table 4: <[D2013] JHHMMSS.sss+DDMMSS.ss> N=708.
=E=	Catalogue in electronic form as J/ApJ/772/131
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2017]
[D2017]	(Davidge, 2017)
Write:	<<[D2017] NN>>
N:	35
Object:	* (SIMBAD class: Star)
Note:	Gemini South GMOS imaging and spectroscopy of N=35 stars in the open cluster NGC 3105.
in source:	NGC 3105
Ref:	=2017ApJ...837..178D
by	DAVIDGE T.J.
	Astrophys. J., 837, 178-178 (2017)
	NGC 3105: a young cluster in the outer galaxy.
o	Table 3: <[D2017] NN> (Nos 1-35).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2017a]
[D2017a]	(Davidge, 2017)
*****	Avoid the usage of [D2017a], prefer [D2017]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2017b]
[D2017b]	(Dewangan, 2017)
Write:	<<[D2017b] NN>>
N:	14
Object:	Clump (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=14 clumps in the molecular cloud GAL 035.2-00.74. Use of archival Herschel continuum maps at 70µm, 160µm, 250µm, 350µm, and 500µm.
in source:	GAL 035.2-00.74
Ref:	=2017ApJ...837...44D
by	DEWANGAN L.K.
	Astrophys. J., 837, 44-44 (2017)
	Star formation activity in the molecular cloud G35.20-0.74: onset of cloud-cloud collision.
o	Fig. 4, Table 2: <[D2017b] NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2019]
[D2019]	(Davidge, 2019)= ([D2019a])
Write:	<<[D2019] HA>> <<[D2019] aNN-NN>>
N:	3+32
Object:	Halpha emitting source + ? (SIMBAD class: EmObj = Emission Object)
Stat.	in SIMBAD: [D2019] HA (Nos HA-HC) not in Simbad
Note:	Gemini South GMOS observations of N=3 Hα sources and N=32 unresolved sources (HII regions, early-type stars, M giants/supergiants, C stars, composite systems, ...), in NGC 55.
in source:	NGC 55
Ref:	=2019AJ....158...90D
by	DAVIDGE T.J.
	Astron. J., 158, 90-90 (2019)
	Changes: the past, present, and future of the nearby dwarf galaxy NGC 55.
o	Figs 5-6: <[D2019] HA> (Nos HA-HC). Table 3: <[D2019] aNN-NN> N=32.
o	2MASS 05284449-6614309 is a misprint for 2MASS J05284449-6614039.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2019a]
[D2019a]	(Davidge, 2019)
*****	Avoid the usage of [D2019a], prefer [D2019]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D2019b]
[D2019b]	(Dewangan, 2019)
Write:	<<[D2019b] Clump NN>> <<[D2019b] Clump A>> <<[D2019b] YSO NNN>>
N:	28+167
Object:	Clump + YSO (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=23+5 clumps and N=167 YSOs in AFGL 5157. Use of data from the following surveys: Extended Outer Galaxy Survey (E-OGS), SCUBA Legacy Catalogues and continuum maps, Herschel Infrared Galactic Plane Survey (Hi-GAL), (WISE), Warm-Spitzer GLIMPSE360 Survey, UGPS, 2MASS, IPHAS.
in source:	RAFGL 5157
Ref:	=2019ApJ...884...84D
by	DEWANGAN L.K.
	Astrophys. J., 884, 84-84 (2019)
	The cluster-forming site AFGL 5157: colliding filamentary clouds and star formation.
o	Fig. 2, Table 2: <[D2019b] Clump NN> (Nos Clump 1-Clump 23). Fig. 3, Table 2: <[D2019b] Clump A> (Nos Clump A-Clump E). Table 3: <[D2019b] YSO NNN> (Nos YSO 1-YSO 167).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D22]
[D22]	(Duncan, 1922)
Write:	<<[D22] N>>
N:	3
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
in source:	M 33 = NGC 598
Ref:	=1922PASP...34..290D
by	DUNCAN J.C.
	Publ. Astron. Soc. Pac., 34, 290-291 (1922)
	Three variable stars and a suspected nova in the spiral nebula M 33 Trianguli.
o	<[D22] N> (Nos 1-3).
Origin	of the Acronym: L (2001AJ....121..870M)
Details on Acronym: D31
D31	(DIRECT survey, M 31)= (DIRECT)
Write:	<<D31 JHHMMSS.s+DDMMSS.s>>
N:	26712
Object:	* (SIMBAD class: Star)
Note:	DIRECT survey for stars in M 31. For variable stars, the authors first used the acronym DIRECT.
in source:	M 31 = NGC 224
Ref:	=2001AJ....122.1383M
by	MOCHEJSKA B.J. , KALUZNY J., STANEK K.Z., SASSELOV D.D.
	Astron. J., 122, 1383-1385 (2001)
	The DIRECT project: catalogs of stellar objects in nearby galaxies. II. Eastern arm and NGC 206 in M31.
o	Tables 1A-1E: <D31 JHHMMSS.s+DDMMSS.s> N=26712.
Ref:	=2003AJ....126..175B
by	BONANOS A.Z. , STANEK K.Z., SASSELOV D.D., MOCHEJSKA B.J., MACRI L.M., KALUZNY J.
	Astron. J., 126, 175-186 (2003)
	DIRECT distances to nearby galaxies using detached eclipsing binaries and cepheids. IX. Variables in the field M31Y discovered with image subtraction.
o	Objects are written with only one '0' in RA, so D31J04413.0+414747.0 is D31 J004413.0+414747.0 for ex. In table 4, [MAP97] 97 is at an incorrect line, it is D31 J004454.0+413145.4.
o	Tables 2-8: <D31 JHHMMSS.s+DDMMSS.s> N=41+126+48+49.
=E=	Catalogue in electronic form as J/AJ/122/1383
=E=	Catalogue in electronic form as J/AJ/126/175
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: D33
D33	(DIRECT survey, M 33)= (DIRECT)
Write:	<<D33 JHHMMSS.s+DDMMSS.s>>
N:	57581
Object:	* (SIMBAD class: Star)
Note:	DIRECT survey for stars in M 33. For variable stars, the authors first used the acronym DIRECT.
in source:	M 33 = NGC 598
Ref:	=2001AJ....121..861M
by	MACRI L.M. , STANEK K.Z., SASSELOV D.D., KROCKENBERGER M., KALUZNY J.
	Astron. J., 121, 861-869 (2001)
	The DIRECT project: catalogs of stellar objects in nearby galaxies. I. The central part of M33.
o	Table 3: <D33 JHHMMSS.s+DDMMSS.s> N=57581.
Ref:	=2001AJ....121..870M
by	MACRI L.M. , STANEK K.Z., SASSELOV D.D., KROCKENBERGER M., KALUZNY J.
	Astron. J., 121, 870-890 (2001)
	DIRECT distances to nearby galaxies using detached eclipsing binaries and cepheids. VI. Variables in the central part of M33.
o	Tables 1-4: <D33 JHHMMSS.s+DDMMSS.s> N=251+47+62+184.
Ref:	=2001AJ....121.2032M
by	MOCHEJSKA B.J. , KALUZNY J., STANEK K.Z., SASSELOV D.D., SZENTGYORGYI A.H.
	Astron. J., 121, 2032-2052 (2001)
	DIRECT distances to nearby galaxies using detached eclipsing binaries and cepheids. VII. Additional variables in the field M33A discovered with image subtraction.
o	(Erratum) Erratum vol. 121, p. 3284
o	Tables 2, 5,8, 10: <D33 JHHMMSS.s+DDMMSS.s> N=45+157+13+41 added.
Ref:	=2001AJ....122.2477M
by	MOCHEJSKA B.J. , KALUZNY J., STANEK K.Z., SASSELOV D.D., SZENTGYORGYI A.H.
	Astron. J., 122, 2477-2489 (2001)
	DIRECT distances to nearby galaxies using detached eclipsing binaries and cepheids. VIII. Additional variables in the field M33B discovered with image subtraction.
o	Tables 1, 4, 7, 9: <D33 JHHMMSS.s+DDMMSS.s> N=89+292+59+391.
=E=	Catalogue in electronic form as J/AJ/121/861
=E=	Catalogue in electronic form as J/AJ/121/870
=E=	Catalogue in electronic form as J/AJ/121/2032
=E=	Catalogue in electronic form as J/AJ/121/2477
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 400d
400d	(400 sq. deg. survey)
*****	Avoid the usage of 400d, prefer [BRT2016]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: 400d
400d	(400 sq. deg. survey)
*****	Avoid the usage of 400d, prefer [TRB2015]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [D59]
[D59]	(Drake)= (D) (Not yet in Simbad)
Write:	<<[D59] NN>>
N:	12
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1959IAUS....9..339D
by	DRAKE F.D.
	IAU Symp., 9 and URSI Symposium 1 held from 30 July to 6 August 1958 Ed. by R.N. Bracewell. Paris symposium on radio astronomy, 9, 339-346 (1959)
	The nature of the radio source Cygnus X.
o	Table I: <[D59] NN> (Nos 1-12)
Details on Acronym: [D61]
[D61]	(De Vaucouleurs, 1961)
Write:	<<[D61] Cloud Wa>> <<[D61] Cloud AWW>> <<[D61] Cloud W'>> <<[D61] Vir R>>
N:	7+5+3
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Structure of the Virgo cluster region. The designation 'Cloud' is used for group of galaxies, and often found in literature as 'W Cloud' instead of 'Cloud W'. The Virgo cluster itself may consist of 2 overlapping, but separate clouds Cloud S and Cloud E, and the 'Virgo Wing' or Cloud W. These clouds are divided in sub-groups S', Wa, Wb, W'. A Southern Extension of Virgo cluster is designated as 'Vir II' containing Clouds V, X, Y. Vir I, II, III represent 3 groups of galaxies: Vir I = Virgo cluster proper. Vir II = Virgo Southern Extension. Vir III = NGC 5846+NGC 5713+NGC 5566. See also [FFS84], BTS87.
in source:	NAME Virgo Cluster
Ref:	=1961ApJS....6..213D
by	DE VAUCOULEURS G.
	Astrophys. J., Suppl. Ser., 6, 213-234 (1961)
	Structure of the Virgo cluster of galaxies.
o	Fig.3, Tables 6, 7: <[D61] Cloud Wa> (Nos E, S, W, Wa, Wb), <[D61] Cloud W'> (Nos S', W'), <[D61] Cloud AWW> (Nos X, V, Y, XNW, XSE).
Ref:	=1973A&A....28..109D
by	DE VAUCOULEURS G. , DE VAUCOULEURS A.
	Astron. Astrophys., 28, 109-118 (1973)
	Apparent distribution and velocities of galaxies in the Virgo cluster and its surroundings.
o	Fig.1: <[D61] Cloud A> (Nos V, Y), <[D61] Vir R> (Nos I-III).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D70]
[D70]	(DuPuy, 1970)
Write:	<<[D70] Haro 31A>> <<[D70] Haro 32A>>
N:	2+9
Object:	G (SIMBAD class: Galaxy)
Note:	Observations at KPNO of [H56] galaxies. [H56] 31 is divided in 2 galaxies. [H56] 32 is an interacting pair (A+B) and there is a cluster of galaxies around [H56] 32 (NAME Haro 32 Cluster) with 9 galaxies A to J.
in source:	[H56] 31
in source:	NAME Haro 32 Cluster
Ref:	=1970AJ.....75.1143D
by	DUPUY D.L.
	Astron. J., 75, 1143-1147 (1970)
	New observations of blue Haro galaxies.
o	Table I: <[D70] Haro 31A> (Nos A-B). Table II: <[D70] Haro 32A> (Nos A-J, I missing).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D71]
[D71]	(Davis, 1971)= (GC)
Write:	<<[D71] HHMM+DDA>>
N:	254
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1971AJ.....76..980D
by	DAVIS M.M.
	Astron. J., 76, 980-992 (1971)
	The NRAO 5-GHz radio source survey. I. A survey of faint sources.
o	Table III: <[D71] HHMM+DDA> N=254
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D72]
[D72]	(Drilling, 1972)
Write:	<<[D72] NN>>
N:	99
Object:	OB* (SIMBAD class: Star)
in source:	NAME NOR REGION
Ref:	=1972AJ.....77..463D
by	DRILLING J.S.
	Astron. J., 77, 463-474 (1972)
	UBV and H β photometry of OB stars in a Milky Way region in Norma.
o	<[D72] NN> N=99
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D73]
[D73]	(Drilling, 1973)
Write:	<<[D73] 3HLF4 NN>> <<[D73] 4HLF4 NN>>
N:	30+32
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Late-type stars in 2 regions at high galactic latitudes. See also [DP70], [PD70]. See also [P67], [DP70], [PD70].
Ref:	=1973AJ.....78...44D
by	DRILLING J.S.
	Astron. J., 78, 44-46 (1973)
	Photoelectric UBV photometry of late-type stars in two regions at high galactic latitude.
o	Late-type stars in 2 regions at high galactic latitudes. Early-type stars in the same region are studied in 1971AJ.....76.1072D: [DP70] and [PD70] in Simbad.
o	Table I: <[D73] 3HLF4 NN> (Nos 1-30). Table II: <[D73] 4HLF4 NN> (Nos 1-32).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D74]
[D74]	(Disney, 1974)
Write:	<<[D74] PKS 0548-322 gN>>
N:	4
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Galaxies in group around PKS 0548-322.
Ref:	=1974ApJ...193L.103D
by	DISNEY M.J.
	Astrophys. J., 193, 103-105 (1974)
	Parkes 0548-322: a BL Lacertae object in a cluster of galaxies.
o	Fig.1, Table 1: <[D74] PKS 0548-322 gn> (Nos g1-g4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D75]
[D75]	(Dolidze, 1975)= ([D75a])
Write:	<<[D75] Np>> <<[D75] NNN>>
N:	7+191
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1975AbaOB..47..171D
by	DOLIDZE M.V.
	Byull. Abastumanskaya Astrofiz. Obs., 47, 171-191 (1975)
	List of probable long-period variables of M types revealed in red light by means of spectral features.
o	List revised and cross-id. by B. Skiff
o	Table 3: <[D75] Np> (Nos 1p-7p), <[D75] NNN> (Nos 1-191)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D75a]
[D75a]	(Dolidze, 1975)
*****	Avoid the usage of [D75a], prefer [D75]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D75b]
[D75b]	(Dolidze, 1975)= (D)
Write:	<<[D75b] Star NN>> <<[D75b] Em* HH+NNN>> <<[D75b] Cl* NN>> <<[D75b] G NN>>
N:	91+1174+11+13
Object:	* + Cluster of * + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 4: N=91 S, C, and MS stars, (Nos 1-91). Table 5: N=1174 Em*. In the format, the '+' sign is used for emission objects already known (with a cross-id.), the'-' sign for new objects, without other id. Table 8: N=11 probable cluster of stars. Table 9: N=13 emssion galaxies. Finding charts coordinates and cross-id. in 2001IBVS.5185....1S.
Ref:	=1975AbaOB..47....3D
by	DOLIDZE M.V.
	Byull. Abastumanskaya Astrofiz. Obs., 47, 3-144 (1975)
	The lists of S, C, MS stars and emission objects revealed in red light observations.
o	Table 4: <[D75b] Star NN> (Nos 1-91). Table 5: <[D75b] Em* HH+NNN> N=1174. Table 8: <[D75b] Cl* NN> (Nos 1-11). Table 9: <[D75b] G NN> (Nos 1-13).
=E=	Catalogue in electronic form as J/other/IBVS/5185
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D76]
[D76]	(Dressler, 1976)
Write:	<<[D76] NNN>>
N:	74
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Numbering from Dressler Ph.D. THesis, University of California, Santa Cruz. This numbering is used in 1989ApJ...336...77F, cross-identified with [FKK89]
in source:	ACO 2256
Ref:	=1989ApJ...336...77F
by	FABRICANT D.G. , KENT S.M., KURTZ M.J.
	Astrophys. J., 336, 77-92 (1989)
	A combined optical/X-ray study of the galaxy cluster Abell 2256.
o	Table 1, col(1): <[FKK89] NNN> (Nos 1-172). Table 1, col(8): <[D76] NNN> N=74 among (Nos 14-486).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D77]
[D77]	(Dyck, 1977)= ([D77a]) = (IRS)
Write:	<<[D77] IRS N>>
N:	2
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Fig.1: Map
in source:	M 8 = Lagoon Nebula
Ref:	=1977AJ.....82..129D
by	DYCK H.M.
	Astron. J., 82, 129-131 (1977)
	Infrared map of M8.
o	<[D77] IRS N> (Nos 1-2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D77a]
[D77a]	(Dyck, 1977)
*****	Avoid the usage of [D77a], prefer [D77]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D77b]
[D77b]	(Denoyelle, 1977) (Not yet in Simbad)
Write:	<<[D77b] NNN>> <<[D77b] NNNN>>
N:	358
Object:	* (SIMBAD class: Star)
Note:	Format NNNN (always a 4 digits one) is used for binary or triple stars (ex.: 1027 and 2027 binary, 1209, 2209, 3209: triple).
Ref:	=1977A&AS...27..343D
by	DENOYELLE J.
	Astron. Astrophys., Suppl. Ser., 27, 343-365 (1977)
	The spatial distribution of young stars in Vela (l=250 to 284).
o	Table 3: <[D77b] NNN> (Nos 1-358), <[D77b] NNNN> always a 4 digits format, N=46.
=E=	Catalogue in electronic form as II/20
=E=	Catalogue in electronic form as <II/20A/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: D80
D80	(D'Odorico+, 1980)
*****	Avoid the usage of D80, prefer DDB
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [D80]
[D80]	(Dressler, 1980)= (Coma) = (D) = (DC)
Write:	<<[D80] ACO NNNN NNNA>> <<[D80] DRCG HHMM+DD NNNA>> <<[D80] Cen NN>> <<[D80] NN-NNN>>
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
in source:	Coma Cluster = ACO 1656
Ref:	=1980ApJS...42..565D
by	DRESSLER A.
	Astrophys. J., Suppl. Ser., 42, 565-609 (1980)
	A catalog of morphological types in 55 rich clusters of galaxies.
o	Table 1: <DRCG HHMM-DD> N=17. Table 2: <[D80] ACO NNNN NNN>, <[D80] DRCG HHMM-DD NNN>, <[D80] CEN NN>, G in 56 ClG, N about 6000.
=E=	Catalogue in electronic form as VII/174
Origin	of the Acronym: L (1996ApJS..106....1W)
Details on Acronym: [D81]
[D81]	(Dressler, 1981)= (D) = ([D81a])
Write:	<<[D81] NN>>
N:	49
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
in source:	ACO 2029
Ref:	=1981ApJ...243...26D
by	DRESSLER A.
	Astrophys. J., 243, 26-31 (1981)
	The dynamics of the cluster of galaxies A 2029.
o	<[D81] NN> (Nos 1-49)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D81a]
[D81a]	(Dressler, 1981)
*****	Avoid the usage of [D81a], prefer [D81]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D81b]
[D81b]	(Dreher, 1981)
Write:	<<[D81b] 3C NNN.N A>> <<[D81b] 3C NNN.N W>> <<[D81b] 3C NNN.N AN>>
N:	23
Object:	Spot in (Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Hotspots in 4 radio-sources: A direction 'W' refers to the entire hotspot, while a letter 'A' refers to a more compact, bright subcomponent. 3C 33: N=1 south hotspot 'S', and N=1 subcomponent 'A' 3C 61.1: N=1 south hotspot 'S', and N=2 subcomponents A and B 3C 234: N=1 east hotspot ''E', and N=1 subcomponent 'A' 3C 390.3: N=7 subcomponents (Nos A-G), with No. C = center component = '[H72] C', N=4 jet knots (Nos J1-J4) in the '[H72] Np' bridge, N=4 knots (Nos N1-N4) in the neck between components B and F, and N=1 counterjet candidate No. L, in the '[H72] Sf' bridge. See also [H72]
in source:	3C 33
in source:	3C 61.1
in source:	3C 234
in source:	3C 390.3
Ref:	=1981AJ.....86..833D
by	DREHER J.W.
	Astron. J., 86, 833-847 (1981)
	High-resolution maps of the hotspots of several class II radio galaxies.
o	Table IV: Spots in Cyg A = '[HR74] A'
o	Table IV: <[D81b] 3C 33 A> N=1, <[D81b] 3C 33 S> N=1., <[D81b] 3C 61.1 A> (Nos A-B), <[D81b] 3C 61.1 S> N=1, <[D81b] 3C 234 A> N=1, <[D81b] 234 E> N=1, <[D81b] 3C 390.3 A> (Nos A-E).
Ref:	=1995MNRAS.277.1097L
by	LEAHY J.P. , PERLEY R.A.
	Mon. Not. R. Astron. Soc., 277, 1097-1114 (1995)
	The jets and hotspots of 3C 390.3.
o	Lobes Np and Sf = '[H72] Np' and '[H72] Sf'
o	<[D81b] 3C 390.3 A> (Nos F, G, L) added. <[D81b] 3C 390.3 AN> (Nos J1-J4, N1-N4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D81c]
[D81c]	(Demin+Dibay+Tomov, 1981) (Not yet in Simbad)
Write:	<<[D81c] NNN>>
N:	105
Object:	Pair of G (SIMBAD class: PairG = Pair of Galaxies)
Ref:	=1981AZh....58..925D
by	DEMIN V.V. , DIBAY E.A., TOMOV A.N.
	Astron. Zh., 58, 925-932 (1981)
	UBV - Photometry of double galaxies. The catalogue.
o	Table 2: <[DDT81] NNN> (Nos 1-105).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D87]
[D87]	(Duerbeck, 1987)
Write:	<<[D87] VNNNN CCC Star N>> <<[D87] A CCC Star N>> <<[D87] AA CCC Star N>> <<[D87] CCC YYYY Star N>>
N:	92
Object:	Star (SIMBAD class: Star)
Note:	Possible ID of the novae.
Ref:	=1987SSRv...45....1D
by	DUERBECK H.W.
	Space Sci. Rev., 45, 1-212 (1987)
	A reference catalogue and atlas of galactic novae.
o	information on 277 objects, mainly classical novae and related objects.
o	<[D87] VNNNN CCC Star N>, <[D87] A CCC Star N>, <[D87] AA CCC Star N>, <[D87] CCC YYYY Star N>, N=92.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D900a]
[D900a]	(Drake, 1990)
*****	Avoid the usage of [D900a], prefer [D90]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D90]
[D90]	(Drake, 1990)= ([D90a])
Write:	<<[D90] N>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=3 radio-sources in the field of sig Ori.
Ref:	=1990AJ....100..572D
by	DRAKE S.A.
	Astron. J., 100, 572-578 (1990)
	Radio-continuum observations of a small sample of hot stars.
o	Table III: <[D90] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D90b]
[D90b]	(Danks, 1990)
Write:	<<[D90b] A>>
N:	5
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Photographic and spectroscopic data of Klemola 11 with the ESO 3.6 telescope at La Silla.
in source:	Klem 11
Ref:	=1990A&A...231...13D
by	DANKS A.C.
	Astron. Astrophys., 231, 13-18 (1990)
	An interacting galaxy in the Klemola 11 group.
o	Figs 1 ,2, Table 3: <[D90b] A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D94]
[D94]	(Doroshenko, 1994)
Write:	<<[D94] M 82 NNN>> <<[D94] SA 68 NN>>
N:	12+17
Object:	* (SIMBAD class: Star)
Note:	Table 1: format 'M 82 NNN', * in the vicinity of M 82, N=12 among (Nos 4-138) Table 2: format 'SA 68 NN', * in the field SA 68, (Nos 1-17)
in source:	SA 68-
in source:	M 82 = NGC 3034
Ref:	=1994PAZh...20..906D
by	DOROSHENKO V.T.
	Pis'ma Astron. Zh., 20, 906-909 (1994)
	UBVR photometry of stars in the vicinity of M 82 and SA 68.
o	K 218 and 280 = SA 68-218 and 280
o	Table 1: <[D94] M 82 NNN> N=12 among (Nos 4-138), Table 2: <[D94] SA 68 NN> (Nos 1-17)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D95]
[D95]	(Da Costa, 1995)
Write:	<<[D95] NNNN>>
N:	96
Object:	* in Cl* (SIMBAD class: Star)
Note:	N=96 among (Nos 162-2097)
in source:	NAME Pyxis Cluster
Ref:	=1995PASP..107..937D
by	DA COSTA G.S.
	Publ. Astron. Soc. Pac., 107, 937-944 (1995)
	C J0907-372 (Pyxis) : a new distant galactic globular cluster.
o	<[D95] NNNN> N=96 among (Nos 162-2097)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D97]
[D97]	(Dickey, 1997)
Write:	<<[D97] ww-NNN>> <<[D97] FF-NNN>>
N:	63
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Table 2: N=63 galaxies detected in HI, Fields 'ne' (northeast), 'ce' (center), and 'sw' (southeast) cover different areas of ACO 2151, while field '47' covers the center of ACO 2147. format 'ne-NNN', 'ce-NNN', 'sw-NNN', N=56 format '47-NNN', N=7 Maps in Figs 5-7, 15-32
in source:	ACO 2151
in source:	ACO 2147
Ref:	=1997AJ....113.1939D
by	DICKEY J.M.
	Astron. J., 113, 1939-1972 (1997)
	A VLA survey of the Hercules cluster. I The HI data.
o	Table 2: <[D97] ww-NNN>, <[D97] 47-NNN> N=63
=E=	Catalogue in electronic form as J/AJ/113/1939
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D98]
[D98]	(Danner, 1998)= ([D98a])
Write:	<<[D98] NN>> <<[D98] RX JHHMM.m+DDMM A>>
N:	89+8
Object:	(X) + Poss. Opt. (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT All-Sky Survey observations Radio and optical counterparts of X-ray sources. 1998A&AS..128..331D: N=89 X-ray sources, (Nos 1-90) No. 41 missing 1998A&AS..128..349D: Possible optical identifications (N=8) for 5 RX sources
Ref:	=1998A&AS..128..331D
by	DANNER R.
	Astron. Astrophys., Suppl. Ser., 128, 331-348 (1998)
	Searching for old neutron stars with ROSAT. I. Soft X-ray sources in molecular clouds at high galactic latitude.
o	Table 2: <[D98] NN> (Nos 1-90) N=89, No. 41 missing
Ref:	=1998A&AS..128..349D
by	DANNER R.
	Astron. Astrophys., Suppl. Ser., 128, 349-357 (1998)
	Searching for old neutron stars with ROSAT. II. Soft X-ray sources in galactic dark clouds.
o	Table 1: Cloud A, B, C = [DT85] Cloud A, B, C. G 317-4 = DCld 317.0-04.1
o	<[D98] RX JHHMM.m+DDMM A> N=8
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D98a]
[D98a]	(Danner, 1998)
*****	Avoid the usage of [D98a], prefer [D98]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [D98b]
[D98b]	(Dehnen, 1998)= (Dehnen)
Write:	<<[D98b] NN>>
N:	14
Object:	Moving Group (SIMBAD class: MouvGroup = Moving Group)
Note:	N=14 moving groups in a sample of more than 14000 nearby stars from the Hipparcos catalog.
Ref:	=1998AJ....115.2384D
by	DEHNEN W.
	Astron. J., 115, 2384-2396 (1998)
	The distribution of nearby stars in velocity space inferred from Hipparcos data.
o	Table 2: <[D98b] NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DA
DA	(D. Allen)
*****	Avoid the usage of DA, prefer [A79]
Origin	of the Acronym: L (2001NewAR..45..135V)
Details on Acronym: DA
DA	(Dominion obs., list A)
Write:	<<DA NNN>>
N:	615
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Ref:	=1968AJ.....73..135G
by	GALT J.A. , KENNEDY J.E.D.
	Astron. J., 73, 135-151 (1968)
	Survey of radio sources observed in the continuum near 1420 MHz, declinations -5 to +70.
o	Table I: <DA NNN> (Nos 1-615)
Details on Acronym: Da
Da	(Dachs)
*****	Avoid the usage of Da, prefer Dachs
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [DA2010]
[DA2010]	(Dewangan+Anandarao, 2010)
Write:	<<[DA2010] sNN>>
N:	17
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Note:	Spitzer IRAC observations of N=17 YSOs in the star-forming region AFGL 437.
in source:	RAFGL 437
Ref:	=2010MNRAS.402.2583D
by	DEWANGAN L.K. , ANANDARAO B.G.
	Mon. Not. R. Astron. Soc., 402, 2583-2590 (2010)
	Spitzer IRAC imaging photometric study of the massive star-forming region AFGL 437.
o	Fig. 2, Table 1: <[DA2010] sNN> (Nos s1-s17).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DA2011]
[DA2011]	(Dewangan+Anandarao, 2011)
Write:	<<[DA2011] JHHMMSS.ss+DDMMSS.s>> <<[DA2011] eNsN>> <<[DA2011] sN>>
N:	86+144+11+50+7+9
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC observations of YSOs in the Sh 2-235 star-forming region.
in source:	SH 2-235
Ref:	=2011MNRAS.414.1526D
by	DEWANGAN L.K. , ANANDARAO B.G.
	Mon. Not. R. Astron. Soc., 414, 1526-1544 (2011)
	Infrared photometric study of the massive star-forming region S235 using Spitzer-Infrared Array Camera and JHK observations.
o	Tables C1-C2, C5-C6: <[DA2011] JHHMMSS.ss+DDMMSS.s> N=86+144+11+50. Figs 4-5, Tables C3-C4: <[DA2011] eNsN> (Nos e1s1-e1s4, e2s1-e2s3). Fig. 10, Tables C7-C8: <[DA2011] sN> (Nos s1-s9).
=E=	Catalogue in electronic form as <J/MNRAS/414/1526/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DA82]
[DA82]	(Duflot-Augarde+Alloin, 1982)
Write:	<<[DA82] Clump A>>
N:	6
Object:	Clump (SIMBAD class: PartofG = Part of a Galaxy)
Note:	N=6 HII-like clumps in NGC 7673
in source:	NGC 7673
Ref:	=1982A&A...112..257D
by	DUFLOT-AUGARDE R. , ALLOIN D.
	Astron. Astrophys., 112, 257-267 (1982)
	Recent star-forming activity in the clumpy irregular galaxy NGC 7673.
o	Fig.1: <[DA82] Clump A> (Nos A-F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DA92]
[DA92]	(Dent+Aspin, 1992)
Write:	<<[DA92] NN>>
N:	31
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	NIPSS 1548C27
Ref:	=1992MNRAS.259..401D
by	DENT W.R.F. , ASPIN C.
	Mon. Not. R. Astron. Soc., 259, 401-409 (1992)
	Molecular and infrared observations of the conical reflection nebula 1548C27.
o	[DA92] 1 = [VMR89] 1, [DA92] 2 = [VMR89] 2
o	<[DA92] NN> N=31
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAA2009]
[DAA2009]	(Diehl+Allam+Annis+, 2009)
Write:	<<[DAA2009] SDSS JHHMMSS.ss+DDMMSS.s>> <<[DAA2009] SDSS JHHMMSS.ss+DDMMSS.s a>> <<[DAA2009] SDSS JHHMMSS.ss+DDMMSS.s source>>
N:	4+10+4
Object:	Grav. lens + Grav. lensed image of a G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Spectroscopy and imaging data from the APO ARC 3.5m telescope of N=4 very bright, strongly lensed galaxies.
Ref:	=2009ApJ...707..686D
by	DIEHL H.T. , ALLAM S.S., ANNIS J., BUCKLEY-GEER E.J., FRIEMAN J.A., KUBIK D., KUBO J.M., LIN H., TUCKER D., WEST A.
	Astrophys. J., 707, 686-692 (2009)
	The Sloan bright arcs survey: four strongly lensed galaxies with redshift > 2.
o	Tables 3-4: <[DAA2009] SDSS JHHMMSS.ss+DDMMSS.s> N=4, <[DAA2009] SDSS JHHMMSS.ss+DDMMSS.s a> N=10, <[DAA2009] SDSS JHHMMSS.ss+DDMMSS.s source> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAB2006]
[DAB2006]	(Djupvik+Andre+Bontemps+, 2006)
Write:	<<[DAB2006] ISO-NNN>> <<[DAB2006] NOT-NNNN>> <<[DAB2006] SIRCA-NN>> <<[DAB2006] MMSN>> <<[DAB2006] MMS1-a>> <<[DAB2006] VLA-N>>
N:	186+1148+46+8+9
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	ISOCAM, NOT ARNICA-SIRCA, IRAM 30m 1.3mm, and VLA 3.6cm observations of the young embedded cluster around CoKU Ser G3 to CoKU Ser G6.
in source:	Serpens Cloud:NAME Serpens G3-G6 Cluster = NAME Serpens G3-G6 Cluster
Ref:	=2006A&A...458..789D
by	DJUPVIK A.A. , ANDRE P., BONTEMPS S., MOTTE F., OLOFSSON G., GALFALK M., FLOREN H.-G.
	Astron. Astrophys., 458, 789-803 (2006)
	A multi-wavelength census of star formation activity in the young embedded cluster around Serpens/G3-G6.
o	Table 1: <[DAB2006] ISO-NNN> (Nos 1 to 186). Table 2: <[DAB2006] NOT-NNNN> (Nos 1 to 1148). Table 3: <[DAB2006] SIRCA-NN> (Nos 1 to 46). Table 7: <[DAB2006] MMSN> (Nos MMS1 to MMS4), <[DAB2006] MMS1-a> (Nos 1-a to 1-d). Table 8: <[DAB2006] VLA-N> (Nos 1 to 9). Text: <NAME Serpens NH3>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAB2006a]
[DAB2006a]	(Djupvik+Andre+Bontemps+, 2006)
*****	Avoid the usage of [DAB2006a], prefer [DAB2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAB2006b]
[DAB2006b]	(Dawson+Aldering+Barbary+, 2006)
Write:	<<[DAB2006b] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	Opt. Transient (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST ACS, Keck LRIS, VLT, and Subaru spectroscopy of a variable object in Bootes.
Ref:	=2006CBET..546....1D
by	DAWSON K. , ALDERING G., BARBARY K., FADEYEV V., GOLDHABER G., GUDE A., HUANG X., KIM A., KOWALSKI M., KUZNETSOVA N., LEE W., MEYERS J., NUGENT P., PERLMUTTER S., RUBIN D., SCHLEGEL D., SPADAFORA T., SUZUKI N., WANG L., DOI M., IHARA Y., MOROKUMA T., TAKANASHI N., TOKITA K., YASUDA N., LIDMAN C., AMANULLAH R., GOOBAR A., STANISHEV V.
	CBET, 546, 1 (2006)
	Variable object in Bootes.
o	<[DAB2006b] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAB2009]
[DAB2009]	(Dye+Ade+Bock+, 2009)= (BLAST)
Write:	<<[DAB2009] NNN>> <<[DAB2009] Rad DDD.ddddd+DD.ddddd>> <<[DAB2009] IR DDD.ddddd+DD.ddddd>>
N:	350
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	Balloon-borne Large Aperture Submillimeter Telescope (BLAST) redshift survey at 250, 350 and 500µm in the GOODS SOUTH FIELD. See also BLAST.
in source:	NAME GOODS South Field
Ref:	=2009ApJ...703..285D
by	DYE S. , ADE P.A.R., BOCK J.J., CHAPIN E.L., DEVLIN M.J., DUNLOP J.S., EALES S.A., GRIFFIN M., GUNDERSEN J.O., HALPERN M., HARGRAVE P.C., HUGHES D.H., KLEIN J., MAGNELLI B., MARSDEN G., MAUSKOPF P., MONCELSI L., NETTERFIELD C.B., OLMI L., PASCALE E., PATANCHON G., REX M., SCOTT D., SEMISCH C., TARGETT T., THOMAS N., TRUCH M.D.P., TUCKER C., TUCKER G.S., VIERO M.P., WIEBE D.V.
	Astrophys. J., 703, 285-299 (2009)
	Radio and mid-infrared identification of BLAST source counterparts in the Chandra Deep Field South.
o	Tables 1-3, col(1): <[DAB2009] NNN> N=351 among (Nos 1-378) = Table 1, col(2): <BLAST JHHMMSS+DDMMSS> N=350. Tables 1-2: <[DAB2009] Rad DDD.ddddd+DD.ddddd>, <[DAB2009] IR DDD.ddddd+DD.ddddd>.
=E=	Catalogue in electronic form as J/ApJ/703/285
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAB2010]
[DAB2010]	(Dunlop+Ade+Bock+, 2010)= (BLAST)
Write:	<<[DAB2010] DDD.dddddd+DD.dddddd>>
N:	27
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA (1.4GHz) radio counterparts for BLAST sources.
in source:	NAME GOODS South Field
Ref:	=2010MNRAS.408.2022D
by	DUNLOP J.S. , ADE P.A.R., BOCK J.J., CHAPIN E.L., CIRASUOLO M., COPPIN K.E.K., DEVLIN M.J., GRIFFIN M., GREVE T.R., GUNDERSEN J.O., HALPERN M., HARGRAVE P.C., HUGHES D.H., IVISON R.J., KLEIN J., KOVACS A., MARSDEN G., MAUSKOPF P., NETTERFIELD C.B., OLMI L., PASCALE E., PATANCHON G., REX M., SCOTT D., SEMISCH C., SMAIL I., TARGETT T.A., THOMAS N., TRUCH M.D.P., TUCKER C., TUCKER G.S., VIERO M.P., WALTER F., WARDLOW J.L., WEISS A., WIEBE D.V.
	Mon. Not. R. Astron. Soc., 408, 2022-2050 (2010)
	The BLAST 250 µm-selected galaxy population in GOODS-south.
o	Table 2: <[DAB2010] DDD.dddddd+DD.dddddd> N=27.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAB2012]
[DAB2012]	(Dunham+Arce+Bourke+, 2012)
Write:	<<[DAB2012] MMSN>>
N:	7 (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	SMA 1.3mm continuum observations of the region of HBC 722.
Ref:	=2012ApJ...755..157D
by	DUNHAM M.M. , ARCE H.G., BOURKE T.L., CHEN X., VAN KEMPEN T.A., GREEN J.D.
	Astrophys. J., 755, 157 (2012)
	Revealing the millimeter environment of the new FU Orionis candidate HBC722 with the submillimeter array.
o	Table 2: <[DAB2012] MMSN> (Nos 1-7)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAB2013]
[DAB2013]	(Duronea+Arnal+Bronfman, 2013)
Write:	<<[DAB2013] aN>> <<[DAB2013] feature N>>
N:	5+4
Object:	MCld + (Rad) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	NANTEN CO(1-0) and 13CO(1-0) observations of the field of WR 16. Use of Parkes-MIT-NRAO Southern Radio Survey archival data at 4.85GHz and of IRAS HIRES 60 and 100µm images.
Ref:	=2013A&A...551A..71D
by	DURONEA N.U. , ARNAL E.M., BRONFMAN L.
	Astron. Astrophys., 551A, 71-71 (2013)
	Carbon monoxide in the environs of the star WR 16.
o	Fig. 2, Table 1: <[DAB2013] aN> (Nos a1-a3, b1-b2). Paragr. 3.2, Fig. 6, Table 2: <[DAB2013] feature N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAB2016]
[DAB2016]	(Del Moro+Alexander+Bauer+, 2013)
Write:	<<[DAB2016] NN>>
N:	33
Object:	QSO (SIMBAD class: QSO = Quasar)
Note:	Spitzer, Herschel and Chandra X-ray observations of N=33 mid-IR luminous quasars at redshift∼1-3 in the GOODS-Herschel North and South fields.
Ref:	=2016MNRAS.456.2105D
by	DEL MORO A. , ALEXANDER D.M., BAUER F.E., DADDI E., KOCEVSKI D.D., McINTOSH D.H., STANLEY F., BRANDT W.N., ELBAZ D., HARRISON C.M., LUO B., MULLANEY J.R., XUE Y.Q.
	Mon. Not. R. Astron. Soc., 456, 2105-2125 (2016)
	Mid-infrared luminous quasars in the GOODS-Herschel fields: a large population of heavily obscured, Compton-thick quasars at z ~ 2.
o	Table 2: <[DAB2016] NN> (Nos 1-33).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAB2020]
[DAB2020]	(Della Bruna+Adamo+Bik+, 2020)
Write:	<<[DAB2020] NGC 7793 SNRN>> <<[DAB2020] NGC 7793 PNN>> <<[DAB2020] NGC 7793 WRN>>
N:	3+2+9
Object:	Poss. SNR + Poss. PN + Poss. WR (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	VLT MUSE observations of N=3 SNR candidates, N=2 PN candidates, and N=9 Wolf-Rayet candidates in NGC 7793.
in source:	NGC 7793
Ref:	=2020A&A...635A.134D
by	DELLA BRUNA L. , ADAMO A., BIK A., FUMAGALLI M., WALTERBOS R., OSTLIN G., BRUZUAL G., CALZETTI D., CHARLOT S., GRASHA K., SMITH L.J., THILKER D., WOFFORD A.
	Astron. Astrophys., 635A, 134-134 (2020)
	Studying the ISM at ~10 pc scale in NGC 7793 with MUSE. I. Data description and properties of the ionised gas.
o	(Erratum) erratum vol. 652, art. C6 (2021)
o	Figs 10-11, Table 2: <[DAB2020] NGC 7793 SNRN> (Nos SNR1-SNR3), <[DAB2020] NGC 7793 PNN> (Nos PN1-PN2), <[DAB2020] NGC 7793 WRN> (Nos WR1-WR9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAB77]
[DAB77]	(Doxsey+Apparao+Bradt+, 1977)
Write:	<<[DAB77] 2S HHMM+DDd NN>> <<[DAB77] 2S HHMM+DDd A>> <<[DAB77] 2S HHMM+DDd AW>> <<[DAB77] 2S HHMM+DDd AWw>>
N:	27+95
Object:	* (SIMBAD class: Star)
Note:	Finding charts in Figs '2S 1837+049 D' is Davidsen's candidate from 1975IAUC.2824....1D Components 'DN' 'DS' 'DSe' and 'DSw' are added in 1997 '2S 1908+005 D' is Davidsen's candidate from 1976ApJ...203..448D '2S 1957+115 M' is Margon's candidate (ref. not found)
Ref:	=1977Natur.269..112D
by	DOXSEY R.E. , APPARAO K.M.V., BRADT H.V., DOWER R.G., JERNIGAN J.G.
	Nature, 269, 112-116 (1977)
	Positions of galactic X-ray sources.
o	Table 2 and Fig1: <[DAB77] 2S 1822-000 N> (Nos 1-5), <[DAB77] 2S 1837+049 NN> (Nos 1-11), <[DAB77] 2S 1837+049 D>, <[DAB77] 2S 1845-024 N> (Nos 1-4), <[DAB77] 2S 1905+000 NN> (Nos 1-26), <[DAB77] 2S 1908+005 NN> (Nos 1-15), <[DAB77] 2S 1908+005 D>, <[DAB77] 2S 1916-053 NN> (Nos 1-20), <[DAB77] 2S 1957+115 NN> (Nos 1-12), <[DAB77] 2S 1957+115 M>.
Ref:	=1977Natur.270..586D
by	DOXSEY R.E. , APPARAO K.M.V., BRADT H.V., DOWER R.G., JERNIGAN J.G.
	Nature, 270, 586-588 (1977)
	Positions of galactic X-ray sources.
o	Nos D and E in 2S 1728-169 = [MPP74] 3U 1728-16 D and E. Nos 'NN' in 2S 1813-140 = [KOS70] GX 17+2 NN, No. 'TR' in 2S 1813-140 = [KOS70] GX 17+2 28.
o	Fig.2: <[DAB77] 2S 1728-247 NN> (Nos 1-14), <[DAB77] 2S 1728-169 N> (Nos 1-8), <[DAB77] 2S 1811-171 N> (Nos 1-5). Fig.2: [KOS70] GX 3+1 NN> (Nos 35-39) added, [KOS70] GX 9+1 NN> (Nos 26-28, 31, 34) added.
Ref:	=1997ApJ...490..401W
by	WACHTER S.
	Astrophys. J., 490, 401-406 (1997)
	New results for two optically faint low-mass X-ray binary systems.
o	Table 2: Nos 5 and 2 = [JAB78] 2S 1702-363 5 and 2. GX 349+2 = 2S 1702-363.
o	Table 2: <[W97] GX 349+2 VN> (Nos V1-V2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAB78]
[DAB78]	(Dower+Apparao+Bradt+, 1978)
Write:	<<[DAB78] 2S HHMM+DDd NNa>>
N:	6+31+4+32+17+38+12
Object:	* (SIMBAD class: Star)
Note:	Stars in the field of N=7 2S sources. Finding charts in Figs
Ref:	=1978Natur.273..364D
by	DOWER R.G. , APPARAO K.M.V., BRADT H.V., DOXSEY R.E., JERNIGAN J.G., KULIK J.
	Nature, 273, 364-367 (1978)
	Positions of galactic X-ray sources : 55 <lII<320.
o	'2S 0614+91 A' = '[MPP74] 0614+91 A', '2S 1254-690 A' = '[PPM75] 3U 1254-69 A', 2S 1258-613 MMV = NAME MMV STAR.
o	Table 2, charts: <[DAB78] 2S 0114+650 N> (Nos 1-6), <[DAB78] 2S 0142+614 NN> (Nos 1-13), <[DAB78] 2S 0614+091 N> (Nos 1-4), <[DAB78] 2S 0918-549 NN> (Nos 1-32), <[DAB78] 2S 1239-599 NN> (Nos 1-17), <[DAB78] 2S 1254-690 NN> (Nos 1-38), <[DAB78] 2S 1258-613 NN> (Nos 1-12).
Ref:	=1998MNRAS.299..223C
by	COE M.J. , PIGHTLING S.L.
	Mon. Not. R. Astron. Soc., 299, 223-228 (1998)
	Deep infrared and optical studies of the fields of three proposed TZO remnants.
o	Fig1, Table 1: Objects are [FHR82] A or [FHR82] RN.
o	Fig2, Table 2: <[DAB78] 2S 0142+614 NNa> (No. 2a) and N=5 among (Nos 14-30) added. Fig3, Table 3: <[CP98] RX J1838.4-0301 A> (Nos A-M), No. I missing.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAB94]
[DAB94]	(Deharveng+Albrecht+Barbieri+, 1994)
Write:	<<[DAB94] NNN>>
N:	145
Object:	* (SIMBAD class: Star)
in source:	ZW I 36
Ref:	=1994A&A...288..413D
by	DEHARVENG J.-M. , ALBRECHT R., BARBIERI C., BLADES J.C., BOKSENBERG A., CRANE P., DISNEY M.J., JAKOBSEN P., KAMPERMAN T.M., KING I.R., MACCHETTO F., MacKAY C.D., PARESCE F., WEIGELT G., BAXTER D., GREENFIELD P., JEDRZEJEWSKI R., NOTA A., SPARKS W.B.
	Astron. Astrophys., 288, 413-424 (1994)
	The massive star content of the blue dwarf galaxy IZw 36 from Faint Object Camera observations.
o	<[DAB94] NNN> N=145
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAC2007]
[DAC2007]	(Diaz-Santos+Alonso-Herrero+Colina+, 2007)
Write:	<<[DAC2007] CNN>>
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST multiwavelength images of NGC 7469. Search of stellar clusters.
in source:	NGC 7469
Ref:	=2007ApJ...661..149D
by	DIAZ-SANTOS T. , ALONSO-HERRERO A., COLINA L., RYDER S.D., KNAPEN J.H.
	Astrophys. J., 661, 149-164 (2007)
	Resolving the stellar populations in the circumnuclear ring of NGC 7469.
o	Table 2: <[DAC2007] CNN> (Nos C1-C30).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAC2011]
[DAC2011]	(Durret+Adami+Cappi+, 2011) (Not yet in Simbad)
Write:	<<[DAC2011] WN-NNNN>>
N:	6802
Object:	Poss. Cluster of G (SIMBAD class: ClG_Candidate = Cluster of Galaxies Candidate)
Note:	N=6802 galaxy cluster candidates in the range 0.1≤z≤1.15, in the CFHTLS Wide survey, based on the T0006 data release. See also [SMD2018] for galaxy cluster candidates in the CFHTLS Wide T0007 data release.
Ref:	=2011A&A...535A..65D
by	DURRET F. , ADAMI C., CAPPI A., MAUROGORDATO S., MARQUEZ I., ILBERT O., COUPON J., ARNOUTS S., BENOIST C., BLAIZOT J., EDORH T.M., GARILLI B., GUENNOU L., LE BRUN V., LE FEVRE O., MAZURE A., McCRACKEN H.J., MELLIER Y., MEZRAG C., SLEZAK E., TRESSE L., ULMER M.P.
	Astron. Astrophys., 535A, 65-65 (2011)
	Galaxy cluster searches based on photometric redshifts in the four CFHTLS wide fields.
o	<[DAC2011] WN-NNNN> (Nos W1-1 to W1-3247, W2-1 to W2-919, W3-1 to W3-1819, W4-1 to W4-817).
=E=	Catalogue in electronic form as <J/A+A/535/A65/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Dachs
Dachs	(Dachs)= (D) = (Da)
Write:	<<Dachs SMC N-NN>> <<Dachs LMC N-NNA>>
N:	23+64+31+35+35
Object:	* (SIMBAD class: Star)
Note:	1st ref.: Stars in 3 fields 1 to 3 in the SMC: field 1: format 'SMC 1-NN', (Nos 1-23) field 2: format 'SMC 2-NN', (Nos 1-64) field 3: format 'SMC 3-NN', (Nos 1-31) 2nd ref.: Stars in 2 fields 1, 2 in the LMC: field 1: format 'LMC 1-NN', (Nos 1-35) field 2: format 'LMC 2-NNA', (Nos 1-33), and Nos 7B, 25B
in source:	Magellanic Clouds:SMC = SMC
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1970A&A.....9...95D
by	DACHS J.
	Astron. Astrophys., 9, 95-109 (1970)
	Photometry of bright stars in the Small Magellanic Cloud.
o	<Dachs SMC 1-NN> (Nos 1-23), <Dachs SMC 2-NN> (Nos 1-64), <Dachs SMC 3-NN> (Nos 1-31)
Ref:	=1972A&A....18..271D
by	DACHS J.
	Astron. Astrophys., 18, 271-286 (1972)
	Photometry of bright stars in the Large Magellanic Cloud.
o	Table 1: <Dachs LMC 1-NN> (Nos 1-35), Table 2: <Dachs LMC 2-NNA> (Nos 1-33) and Nos 7B, 25B
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAF68]
[DAF68]	(De Vaucouleurs+Angione+Fraser, 1968)
Write:	<<[DAF68] A>> <<[DAF68] AN>> <<[DAF68] AW>> <<[DAF68] AW-W>> <<[DAF68] AA>>
N:	24
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Structure of the jet in M 87. Since 1956 (see [B56]), and along the years, N=11 knots are defined, (Nos A-K), knots B, C and G being divided into 2 components (Nos B1-B2, C1-C2, G1-G2), with B2= K and [DAF68] A to C = [B56] A to C. N=1 Filament (No. L), and the nucleus or central source (No. S). Knot [DAF68] D has 3 components (Nos DE, DM, DW), N=1 sub-component to DE: DE-W, and N=1 Chandra X-ray component DX. The HST has permitted to add new knots, [PBZ99].
in source:	M 87 = NGC 4486 = Virgo A
Ref:	=1968ApL.....2..141D
by	DE VAUCOULEURS G. , ANGIONE R., FRASER C.W.
	Astrophys. Lett., 2, 141-146 (1968)
	Detailed photometry of the jet in Messier 87.
o	Table III: <[DAF68] A> (Nos A-H).
Ref:	=1979ApJ...231..364D
by	DE VAUCOULEURS G. , LIETO J.-L.
	Astrophys. J., 231, 364-371 (1979)
	A photometric analysis of the jet in Messier 87.
o	Table 2: <[DAF68] A> (Nos I-K, S) added.
Ref:	=1983CR2...296.1779L
by	LELIEVRE G. , NIETO J.-L., WLERICK G., SERVAN B., RENARD L., HORVILLE D.
	C.R. Acad. Sci. Ser. II, 296, 1779-1786 (1983)
	Systemes extra-galactiques. -Etude, a haute resolution, du jet optique de Messier 87.
o	Table II: <[DAF68] A> (No. L) added.
Ref:	=1996ApJ...473..254S
by	SPARKS W.B. , BIRETTA J.A., MACCHETTO F.
	Astrophys. J., 473, 254-268 (1996)
	The jet of M87 at tenth-arcsecond resolution: optical, ultraviolet, and radio observations.
o	Table 3: <[DAF68] AN> (Nos B1-B2) added.
Ref:	=1999AJ....117.2185P
by	PERLMAN E.S. , BIRETTA J.A., ZHOU F., SPARKS W.B., MACCHETTO F.D.
	Astron. J., 117, 2185-2198 (1999)
	Optical and radio polarimetry of the M87 jet at 0".2 resolution.
o	Figs 2, 5: regions HOP and LOP not in SIMBAD.
o	Fig.1: <[PBZ99] HST-1> N=1. Fig.6: <[DAF68] AN> (Nos G1-G2) added.
Ref:	=1999ApJ...520..621B
by	BIRETTA J.A. , SPARKS W.B., MACCHETTO F.
	Astrophys. J., 520, 621-626 (1999)
	Hubble space telescope observations of superluminal motion in the M87 jet.
o	Knots 'A' = [DAF68] A
o	Table 2: <[PBZ99] HST-N> (No. 2) added, <[PBZ99] HST-1 East> N=1, <[PBZ99] HST-1 aaa> (Nos alp to eps) N=5. Table 2: <[DAF68] DW> (Nos DE, DM, DW), <[DAF68] DE-W> N=1.
Ref:	=2001ApJ...551..206P
by	PERLMAN E.S. , BIRETTA J.A., SPARKS W.B., MACCHETTO F.D., LEAHY J.P.
	Astrophys. J., 551, 206-222 (2001)
	The Optical-Near-Infrared spectrum of the M87 jet from Hubble Space Telescope observations.
o	Table 2: <[DAF68] AN> (Nos C1-C2) added.
Ref:	=2002ApJ...564..683M
by	MARSHALL H.L. , MILLER B.P., DAVIS D.S., PERLMAN E.S., WISE M., CANIZARES C.R., HARRIS D.E.
	Astrophys. J., 564, 683-687 (2002)
	A high-resolution X-ray image of the jet in M87.
o	Table 1 : Knots "A" are [DAF68], HST-1 = [PBZ99] HST-1
o	Table 1: <[DAF68] DX> N=1 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAG2006]
[DAG2006]	(Dominici+Abraham+Galo, 2006) (Not yet in Simbad)
Write:	<<[DAG2006] PKS 2005-489 N>> <<[DAG2006] PKS 2005-489 G>> <<[DAG2006] PKS 2155-304 N>>
N:	4+1+6
Object:	* (SIMBAD class: Star)
Note:	Stars in the field of 2 BL LLacs.
Ref:	=2006A&A...460..665D
by	DOMINICI T.P. , ABRAHAM Z., GALO A.L.
	Astron. Astrophys., 460, 665-672 (2006)
	Optical and near-infrared simultaneous observations of the BL Lacs PKS 2005-489 and PKS 2155-304.
o	Fig.1: <[DAG2006] PKS 2005-489 N> (Nos 1-4), <[DAG2006] PKS 2005-489 G> N=1, <[DAG2006] PKS 2155-304 N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAG2016]
[DAG2016]	(Dahle+Aghanim+Guennou+, 2016)
Write:	<<[DAG2016] PSZ1-ARC G311.6602-18.4624>> <<[DAG2016] PSZ1 G311.65-18.48 SN>> <<[DAG2016] PSZ1 G311.65-18.48 source>> <<[DAG2016] PSZ1 G311.65-18.48 BCG>>
N:	1+3+1+1
Object:	Grav. lens system + Grav. lensed image of a G + Grav. lensed image + EmG + Brightest Cluster Galaxy (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	ESO NTT EFOSC2 and Magellan-I Baade Telescope IMACS observations of N=1 graivational lens system, N=1 gravitationally lensed arc with N=3 brighter segments of N=1 background LAE in the field of PSZ1 G311.65-18.48.
Ref:	=2016A&A...590L...4D
by	DAHLE H. , AGHANIM N., GUENNOU L., HUDELOT P., KNEISSL R., POINTECOUTEAU E., BEELEN A., BAYLISS M., DOUSPIS M., NESVADBA N., HEMPEL A., GRONKE M., BURENIN R., DOLE H., HARRISON D., MAZZOTTA P., SUNYAEV R.
	Astron. Astrophys., 590L, 4-4 (2016)
	Discovery of an exceptionally bright giant arc at z = 2.369, gravitationally lensed by the Planck cluster PSZ1 G311.65-18.48.
o	<[DAG2016] PSZ1-ARC G311.6602-18.4624> N=1, <[DAG2016] PSZ1 G311.65-18.48 SN> (Nos S1-S3), <[DAG2016] PSZ1 G311.65-18.48 source> N=1, <[DAG2016] PSZ1 G311.65-18.48 BCG> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAL2002]
[DAL2002]	(Durret+Adami+Lobo, 2002)
Write:	<<[DAL2002] NNNNN>>
N:	37058
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	ACO 496
Ref:	=2002A&A...393..439D
by	DURRET F. , ADAMI C., LOBO C.
	Astron. Astrophys., 393, 439-444 (2002)
	Environmental effects on the galaxy luminosity function in the cluster of galaxies Abell 496.
o	Catalog: <[DAL2002] NNNNN> (Nos 1-37058).
=E=	Catalogue in electronic form as J/A+A/393/439
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAL2005]
[DAL2005]	(De Frijs+Anders+Lamers+, 2005) (Not yet in Simbad)
Write:	<<[DAL2005] GN-NN>>
N:	17+20
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	HST imaging observations of star clusters systems. Sample of galaxies in NGC 3310 and NGC 4038/39 clusters.
in source:	NGC 3310
in source:	NAME the Antennae
Ref:	=2005MNRAS.359..874D
by	DE GRIJS R. , ANDERS P., LAMERS H.J.G.L.M., BASTIAN N., FRITZE-v.ALVENSLEBEN U., PARMENTIER G., SHARINA M.E., YI S.
	Mon. Not. R. Astron. Soc., 359, 874-894 (2005)
	Systematic uncertainties in the analysis of star cluster parameters based on broad-band imaging observations.
o	Table 1: <[DAL2005] G1-NN> (Nos G1-01 to G1-17). Table 21: <[DAL2005] G2-NN> (Nos G2-01 to G2-20).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAL2019]
[DAL2019]	(Deras+Arellano Ferro+Lazaro+, 2019)
Write:	<<[DAL2019] M13 CNN>>
N:	15
Object:	Poss. V* (SIMBAD class: Variable*_Candidate = Variable Star Candidate)
Stat:	is completely incorporated in Simbad
Note:	Indian Astronomical Observatory (IAO) 2.0-m telescope and IAC 0.80-m telescope observations of N=15 variable star candidates in M13. See also Cl* NGC 6205 SAW.
in source:	NGC 6205 = M 13
Ref:	=2019MNRAS.486.2791D
by	DERAS D. , ARELLANO FERRO A., LAZARO C., BUSTOS FIERRO I.H., CALDERON J.H., MUNEER S., GIRIDHAR S.
	Mon. Not. R. Astron. Soc., 486, 2791-2808 (2019)
	A new study of the variable star population in the Hercules globular cluster (M13: NGC 6205).
o	Fig. 2, Table 2: <Cl* NGC 6205 SAW VNN> (Nos V54-V60) added. Fig. 2, Table 3: <[DAL2019] M13 CNN> (Nos C1-C15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAL2020]
[DAL2020]	(Deras+Arellano Ferro+Lazaro+, 2020)
Write:	<<[DAL2020] NGC 6712 FV N>> <<[DAL2020] NGC 6712 C>>
N:	9+1
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	IAC 0.80-m telescope and Indian Astronomical Observatory (IAO) 2.0-m telescope photometric observations of N=9+1 variable stars in NGC 6712. Use of Gaia DR2 data. See also Cl* NGC 6205 SAW.
in source:	NGC 6712
Ref:	=2020MNRAS.493.1996D
by	DERAS D. , ARELLANO FERRO A., LAZARO C., BUSTOS FIERRO I.H., CALDERON J.H., MUNEER S., GIRIDHAR S.
	Mon. Not. R. Astron. Soc., 493, 1996-2014 (2020)
	NGC 6712: the variable star population of a tidally disrupted globular cluster.
o	Table 3: <Cl* NGC 6712 SAW VNN> (Nos V30-V36) added, <[DAL2020] NGC 6712 C> N=1. Table 4: <[DAL2020] NGC 6712 FVN> (Nos FV1-FV9).
=E=	Catalogue in electronic form as <J/MNRAS/493/1996/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAM2004]
[DAM2004]	(Di Francesco+Andre+Myers, 2004)
Write:	<<[DAM2004] Oph A-NN>>
N:	6
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	BIMA and IRAM 30m telescope N2H+ (1-0) line observations of the Rho Oph A core.
in source:	NAME rho Oph A
Ref:	=2004ApJ...617..425D
by	DI FRANCESCO J. , ANDRE P., MYERS P.C.
	Astrophys. J., 617, 425-438 (2004)
	Quiescent dense gas in protostellar clusters: the Ophiuchus A core.
o	(Erratum) erratum vol. 700, p. 1994 (2009)
o	p.427 radio sources J1625-254 = RORF 1622-253, J1733-130 = RORF 1730-130
o	Table 1: <[DAM2004] Oph A-AN> (Nos A-N1 to A-N6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAM86]
[DAM86]	(Dodd+Andrews+MacGillivray, 1986)
Write:	<<[DAM86] NNN>>
N:	127
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
in source:	NAME SHAPLEY-CEN CL
Ref:	=1986Ap&SS.122...63D
by	DODD R.J. , ANDREWS F.P., MacGILLIVRAY H.T.
	Astrophys. Space Sci., 122, 63-72 (1986)
	Static properties of galaxies in the Shapley-Centaurus cluster. I. The catalogue.
o	<NAME SHAPLEY-CENTAURUS CL>. Table 1: <[DAM86] NNN> (Nos 1-127)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DANCe
DANCe	(Dynamical Analysis of Nearby Clusters)
Write:	<<DANCe JHHMMSSss+DDMMSSs>>
N:	about 30.10⁶
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	The DANCe surveys measured proper motions by combining archival and new wide field images. The main scientific goal of the survey focuses on nearby associations and clusters, but the catalogs include the astrometry, multi-wavelength (optical and near-infrared) photometry for millions of sources in the field of view. The survey encompasses areas of typically 5 to 100 square degrees around each cluster, and reaches optical magnitudes of the order of 24mag. The accuracy on the proper motion reaches 0.3mas/yr in the best cases, depending on the observational history. Website: http://project-dance.com
in source:	NAME Pleiades
in source:	NGC 2168 = M 35
in source:	NAME VI CYG = Ass Cyg OB 2
Ref:	=2015A&A...575A.120B
by	BOUY H. , BERTIN E., BARRADO D., SARRO L.M., OLIVARES J., MORAUX E., BOUVIER J., CUILLANDRE J.-C., RIBAS A., BELETSKY Y.
	Astron. Astrophys., 575A, 120-120 (2015)
	Messier 35 (NGC 2168) DANCe. I. Membership, proper motions, and multiwavelength photometry.
o	Table 3: <DANCe JHHMMSSss+DDMMSSs> N=337522.
Ref:	=2015A&A...577A.148B
by	BOUY H. , BERTIN E., SARRO L.M., BARRADO D., MORAUX E., BOUVIER J., CUILLANDRE J.-C., BERIHUETE A., OLIVARES J., BELETSKY Y.
	Astron. Astrophys., 577A, 148-148 (2015)
	The Seven Sisters DANCe. I. Empirical isochrones, luminosity, and mass functions of the Pleiades cluster.
o	<DANCe JHHMMSSss+DDMMSSs> N=1969890.
Ref:	=2016MNRAS.460.2593W
by	WRIGHT N.J. , BOUY H., DREW J.E., SARRO L.M., BERTIN E., CUILLANDRE J.-C., BARRADO D.
	Mon. Not. R. Astron. Soc., 460, 2593-2610 (2016)
	Cygnus OB2 DANCe: A high-precision proper motion study of the Cygnus OB2 association.
o	Table 2: <DANCe JHHMMSSss+DDMMSSs> N=873. CAB CSIC
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: DANCe
DANCe	(Dynamical Analysis of Nearby Clusters)
*****	Avoid the usage of DANCe, prefer [SBB2014]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Danks
Danks	(Danks)
Write:	<<Cl Danks N>>
N:	2
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	Cl Danks 1 = C 1309-624, Cl Danks 2 = C 1310-624
Ref:	=1984A&AS...58..163L
by	LUNDSTROM I. , STENHOLM B.
	Astron. Astrophys., Suppl. Ser., 58, 163-192 (1984)
	Wolf-Rayet stars in open clusters and associations.
o	<Cl Danks N> (Nos 1-2)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: DAO
DAO	(Dominion Astroph. Obs.)
*****	Avoid the usage of DAO, prefer [CCS85]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: DASCH
DASCH	(Digital Access to a Sky Century at Harvard)
Write:	<<DASCH JHHMMSS.s+DDMMSS>>
N:	4
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Variable stars found in the Digital Access to a Sky Century at Harvard project.
Ref:	=2010ApJ...710L..77T
by	TANG S. , GRINDLAY J., LOS E., LAYCOCK S.
	Astrophys. J., 710L, 77-81 (2010)
	DASCH discovery of large amplitude ~10-100 year variability in K giants.
o	<DASCH JHHMMSS.s+DDMMSS> N=3.
Ref:	=2012ApJ...751...99T
by	TANG S. , GRINDLAY J.E., MOE M., OROSZ J.A., KURUCZ R.L., QUINN S.N., SERVILLAT M.
	Astrophys. J., 751, 99 (2012)
	DASCH discovery of a possible nova-like outburst in a peculiar symbiotic binary.
o	<DASCH JHHMMSS.s+DDMMSS> N=1 added.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DAT2000]
[DAT2000]	(Diaz+Alvarez+Terlevich+, 2000) (Not yet in Simbad)
Write:	<<[DAT2000] NGC NNNN NN>> <<[DAT2000] NGC 1068 A>>
N:	68
Object:	HII (SIMBAD class: HIIReg = HII Region)
in source:	NGC 1068
in source:	NGC 3310
in source:	NGC 7177
in source:	NGC 7469
Ref:	=2000MNRAS.311..120D
by	DIAZ A.I. , ALVAREZ M.A., TERLEVICH E., TERLEVICH R., SANCHEZ PORTAL M., ARETXAGA I.
	Mon. Not. R. Astron. Soc., 311, 120-134 (2000)
	V, R, I and Hα photometry of circumnuclear star-forming regions in four galaxies with different levels of nuclear activity.
o	Table 4: <[DAT2000] NGC 1068 NN> (Nos 1-23), <[DAT2000] NGC 1068 A> (Nos A-B), <[DAT2000] NGC 3310 NN> (Nos 1-21), <[DAT2000] NGC 7177 NN> (Nos 1-11), <[DAT2000] NGC 7469 NN> (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DAT2004]
[DAT2004]	(Dominici+Abraham+Teixeira+, 2004)
Write:	<<[DAT2004] PKS HHMM+DDd AN>>
N:	3+4
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 2: references stars 'CN' used for PKS 2005-489 and PKS 2155-304 observations.
Ref:	=2004AJ....128...47D
by	DOMINICI T.P. , ABRAHAM Z., TEIXEIRA R., BENEVIDES-SOARES P.
	Astron. J., 128, 47-55 (2004)
	Long-term optical variability of the blazars PKS 2005-489 and PKS 2155-304.
o	Table 2: <[DAT2004] PKS 2005-489 CN> (Nos C1-C3), <[DAT2004] PKS 2155-304 CN> (Nos C1-C4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DAY-I
DAY-I	(Day I)
Write:	<<DAY-I CHHMM+DDd-NNNNN>>
N:	842
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Multicolor photometry with the YALO telescope at the CTIO. Observations of 10 star clusters.
in source:	C 0718-218 = NGC 2367
in source:	C 1033-579 = NGC 3293
in source:	C 1041-597 = Cl Collinder 228
in source:	C 1108-601 = Cl Hogg 10
in source:	C 1109-601 = Cl Hogg 11
in source:	C 1109-604 = Cl Trumpler 18
in source:	C 1110-605 = NGC 3590
in source:	C 1204-609 = NGC 4103
in source:	C 1227-645 = NGC 4463
in source:	C 1424-594 = NGC 5606
Ref:	=2007A&A...467.1397D
by	DELGADO A.J. , ALFARO E.J., YUN J.L.
	Astron. Astrophys., 467, 1397-1407 (2007)
	Pre-main sequence stars in open clusters. I. The DAY-I catalogue.
o	Catalog: < DAY-I CHHMM+DDd-NNNNN> N=842.
=E=	Catalogue in electronic form as J/A+A/467/1397
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DAZ2013]
[DAZ2013]	(De Grijs+Anders+Zackrisson+, 2013)
Write:	<<[DAZ2013] NNN>>
N:	182
Object:	Poss. Cluster of * (SIMBAD class: Cluster*_Candidate = Cluster of Stars Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=182 extended cluster candidates in NGC 5253. Use of HST archival data.
in source:	NGC 5253
Ref:	=2013MNRAS.431.2917D
by	DE GRIJS R. , ANDERS P., ZACKRISSON E., OSTLIN G.
	Mon. Not. R. Astron. Soc., 431, 2917-2932 (2013)
	The NGC 5253 star cluster system - I. Standard modelling and infrared-excess sources.
o	Tables 2-3: <[DAZ2013] NNN> (Nos 0-181).
=E=	Catalogue in electronic form as <J/MNRAS/431/2917/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DB
DB	(Dodd+Brand) (Not yet in Simbad)
*****	Avoid the usage of DB, prefer [DB76]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: DB
DB	(Dominion obs., list B)
Write:	<<DB NNN>>
N:	124
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1968AJ.....73..717B
by	BRIDLE A.H. , PURTON C.R.
	Astron. J., 73, 717-726 (1968)
	Observations of radio sources at 10.03 MHz.
o	Table I: <DB NNN> (Nos 1-124)
Details on Acronym: Db
Db	(Dearborn obs.)
*****	Avoid the usage of Db, prefer DO
Details on Acronym: DB00
DB00	(Dutra+Bica, 2000)
*****	Avoid the usage of DB00, prefer [DB2000]
Origin	of the Acronym: L (2004ApJ...611..858L)
Details on Acronym: DB01
DB01	(Dutra+Bica, 2001)
*****	Avoid the usage of DB01, prefer [DB2001]
Origin	of the Acronym: L (2004ApJ...611..858L)
Details on Acronym: [DB2000]
[DB2000]	(Dutra+Bica, 2000)= (DB00)
Write:	<<[DB2000] NN>>
N:	58
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	IR search for new star clusters in a field centered close to the galactic nucleus, using 2MASS survey archive. See [DB2001].
in source:	NAME Gal Center
Ref:	=2000A&A...359L...9D
by	DUTRA C.M. , BICA E.
	Astron. Astrophys., 359, 9-12 (2000)
	New star clusters projected close to the Galactic Centre.
o	Table 1: <[DB2000] NN> (Nos 1-58).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DB2001]
[DB2001]	(Dutra+Bica, 2001)= (DB01)
Write:	<<[DB2001] JHHMMSS.s+DDMMSS>> <<[DB2001] Cl NN>> <<[DB2001] IRDN N>>
N:	1+42+5
Object:	Cluster of * + Nebula (SIMBAD class: Infrared = Infra-Red Source)
Note:	Objects detected with 2MASS. Fig.1: N=1 newly found IR nebula 'J203925.9+412002'. N=42 new IR star clusters, stellar group and candidates. N=5 IR Dark Nebula (IRDN).
Ref:	=2001A&A...376..434D
by	DUTRA C.M. , BICA E.
	Astron. Astrophys., 376, 434-440 (2001)
	New infrared star clusters and candidates in the Galaxy detected with 2MASS.
o	Fig.1: <[DB2001] JHHMMSS.s+DDMMSS> N=1. Table 1: <[DB2001] Cl NN> (Nos 1-42). Table 2: <[DB2001] IRDN N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DB2002]
[DB2002]	(Demers+Battinelli+, 2002)= ([DB2002a])
Write:	<<[DB2002] SagDIG CNN>> <<[DB2002] Leo I CNN>>
N:	16+13
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Note:	See also [ADK2000], [BD2000], [LDB2002], [BDL2003], [DBL2003], [DBL2003b], [BD2004a], [BD2004b], [DBL2004].
in source:	NAME Sag dIG
in source:	UGC 5470 = Leo I
Ref:	=2002AJ....123..238D
by	DEMERS S. , BATTINELLI P.
	Astron. J., 123, 238-243 (2002)
	C star survey of local group dwarf galaxies. III. The Sagittarius dwarf irregular and the Leo I dwarf spheroidal galaxies.
o	Table 5: Numbering from Cook K.H. PhD. Thesis, Univ. Arizona, 1987.
o	Table 3: <[DB2002] SagDIG CNN> (Nos C01-C16). Table 4: <[DB2002] Leo I CNN> (Nos C01-C13). Table 5: <[C87b] NN> (Nos 1-26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DB2002a]
[DB2002a]	(Demers+Battinelli+, 2002)
*****	Avoid the usage of [DB2002a], prefer [DB2002]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DB2002b]
[DB2002b]	(Dutra+Bica, 2002)
Write:	<<[DB2002b] GLLL.ll+BB.bb>>
Object:	Dust Cloud (SIMBAD class: DarkNeb = Dark Cloud (nebula))
Note:	Compilation of 21 catalogues of dust clouds.
Ref:	=2002A&A...383..631D
by	DUTRA C.M. , BICA E.
	Astron. Astrophys., 383, 631-635 (2002)
	A catalogue of dust clouds in the Galaxy.
o	in ref list CHURCHWELL 1978A&A....67..139C instead of A&AS.67.139
o	Catalog: <[DB2002b] GLLL.ll+BB.bb> N=5004.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DB2005]
[DB2005]	(Demers+Battinelli, 2005)
Write:	<<[DB2005] NNN>>
N:	463
Object:	C* (SIMBAD class: C* = Carbon Star)
Note:	CFHT Megacam camera is used to survey the southern outer disc of M 31, to identify Carbon star candidates.
in source:	M 31 = NGC 224
Ref:	=2005A&A...436...91D
by	DEMERS S. , BATTINELLI P.
	Astron. Astrophys., 436, 91-99 (2005)
	The C star outer disk population of M31 seen with the SLOAN filters.
o	Table 2: <[DB2005] NNN> (Nos 1-463).
=E=	Catalogue in electronic form as J/A+A/436/91
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DB2007]
[DB2007]	(Demers+Battinelli, 2007)
Write:	<<[DB2007] NNN>>
N:	103
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Spectroscopic observations with the 1.8m Plaskett Telescope at the Dominion Astrophysical Observatory.
Ref:	=2007A&A...473..143D
by	DEMERS S. , BATTINELLI P.
	Astron. Astrophys., 473, 143-148 (2007)
	C stars as kinematic probes of the Milky Way disk from 9 to 15 kpc.
o	Paragr.3: 2259+1749 is a misprint for [TI98] 2259+1249. Tables 1 and 4 contain 103 stars; only 76 are confirmed carbon stars, but it is not indicated in the table; thus all objects are finally put as star in Simbad, without spectral type.
o	Table 1: <[DB2007] NNN> (Nos 1-103).
=E=	Catalogue in electronic form as J/A+A/473/143
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DB76]
[DB76]	(Dodd+Brand, 1976)= (DB)
Write:	<<[DB76] FFF-NN>>
N:	29
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Rem:	Identif. charts
Ref:	=1976A&AS...25..519D
by	DODD R.J. , BRAND P.W.J.L.
	Astron. Astrophys., Suppl. Ser., 25, 519-525 (1976)
	A catalogue of galaxies near the galactic plane between l=245 and l=255.
o	<[DB76] FFF-NN> N=29
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DB98]
[DB98]	(Desmurs+Baudry, 1998) (Not yet in Simbad)
Write:	<<[DB98] M17 A>> <<[DB98] ON1 A>> <<[DB98] ON1 A'>> <<[DB98] W51 A>>
N:	8
Object:	OH Maser (SIMBAD class: Maser)
in source:	M 17 = NGC 6618
in source:	Onsala 1
in source:	W 51
Ref:	=1998A&A...340..521D
by	DESMURS J.F. , BAUDRY A.
	Astron. Astrophys., 340, 521-526 (1998)
	VLBI observations of 6 GHz OH masers in three ultra-compact HII regions.
o	Table 2: <[DB98] M17 A> (Nos A-B), <[DB98] ON1 A> (Nos A-D), <[DB98] ON1 A'> (No. A'), <[DB98] W51 A> (No. A).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DB99]
[DB99]	(Devine+Bally, 1999)
Write:	<<[DB99] A>>
N:	9
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Search for H-alpha emission in M 82. N=9 H-alpha bright knots (Nos A-I). Map in Fig.2
in source:	M 82 = NGC 3034
Ref:	=1999ApJ...510..197D
by	DEVINE D. , BALLY J.
	Astrophys. J., 510, 197-204 (1999)
	Hα emission 11 kiloparsecs above M82.
o	Table 1: <[DB99] A> (Nos A-I).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBA2001]
[DBA2001]	(Daniels+Brosch+Almoznino+, 2001)
Write:	<<[DBA2001] FANN>> <<[DBA2001] FNNNN>>
N:	46+221
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Note:	Faust observations aboard Atlas-1 Shuttle flight, in the direction of The Antennae and NGC 6752. In the format, 'FA' stands for Field Antennae, 'FN' for Field NGC (for NGC 6752)
Ref:	=2001MNRAS.324..580D
by	DANIELS J. , BROSCH N., ALMOZNINO E., SHEMMER O., BOWYER S., LAMPTON M.
	Mon. Not. R. Astron. Soc., 324, 580-598 (2001)
	FAUST observations of ultraviolet sources in the directions of NGC 4038-39 and 6752.
o	Table 1: <[DBA2001] AANNN> (Nos FA1-FA46). Table 2: <[DBA2001] AANNN> N=221 among (Nos FN1-FN752).
=E=	Catalogue in electronic form as J/MNRAS/324/580
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBA2006]
[DBA2006]	(Demers+Battinelli+Artigau, 2006)
Write:	<<[DBA2006] NNNN>>
N:	142
Object:	C* (SIMBAD class: C* = Carbon Star)
Note:	CPAPIR (Camera Panoramique Proche IR) at the CTIO 1.5m telescope search for Carbon stars in NGC 6822. See also [LDB2002].
in source:	NGC 6822
Ref:	=2006A&A...456..905D
by	DEMERS S. , BATTINELLI P., ARTIGAU E.
	Astron. Astrophys., 456, 905-910 (2006)
	Carbon stars in the outer spheroid of NGC 6822.
o	Table 2: <[DBA2006] NNNN> (Nos 1001-1142).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBA98]
[DBA98]	(Dallacasa+Bondi+Alef+, 1998) (Not yet in Simbad)
Write:	<<[DBA98] HHMM+DDd CN>>
N:	56
Object:	Component of QSO (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=51 components format 'CN' of 21 QSO or G format 'HHMM+DDd'
Ref:	=1998A&AS..129..219D
by	DALLACASA D. , BONDI M., ALEF W., MANTOVANI F.
	Astron. Astrophys., Suppl. Ser., 129, 219-236 (1998)
	European VLBI Network dual frequency observations of CSS-GPS candidates.
o	Fig.2, Tables 3-5: <[DBA98] HHMM+DDd CN> N=56
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DBB
DBB	(Desert+Bazell+Boulanger)
*****	Avoid the usage of DBB, prefer IREC
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [DBB2002]
[DBB2002]	(De Heij+Braun+Burton, 2002)
Write:	<<[DBB2002] NNN>> <<[DBB2002] LLL.l+BB.b+VVV>>
N:	916
Object:	HVC (SIMBAD class: HVCld = High-velocity Cloud)
Stat:	is completely incorporated in Simbad
Ref:	=2002A&A...391..159D
by	DE HEIJ V. , BRAUN R., BURTON W.B.
	Astron. Astrophys., 391, 159-178 (2002)
	An automated search for compact high-velocity clouds in the Leiden/Dwingeloo Survey.
o	Table 1, col(1): <[DBB2002] NNN> (Nos 1-917) = Table 1, col(2): <[DBB2002] LLL.l+BB.b+VVV> N=916.
=E=	Catalogue in electronic form as J/A+A/391/159
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBB2016]
[DBB2016]	(De Gregorio-Monsalvo+Barrado+Bouy+, 2016)
Write:	<<[DBB2016] ChaII-APEX-A>>
N:	15
Object:	Core (SIMBAD class: denseCore = Dense Core)
Note:	APEX LABOCA 870µm observations of N=15 cores in the Chamaeleon II molecular cloud.
in source:	NAME Cha II
Ref:	=2016A&A...590A..79D
by	DE GREGORIO-MONSALVO I. , BARRADO D., BOUY H., BAYO A., PALAU A., MORALES-CALDERON M., HUELAMO N., MORATA O., MERIN B., EIROA C.
	Astron. Astrophys., 590A, 79-79 (2016)
	A submillimetre search for pre- and proto-brown dwarfs in Chamaeleon II.
o	Table 2: <[DBB2016] ChaII-APEX-A> (Nos A-O).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
History	of this Acronym: replaced by
Details on Acronym: [DBC2001]
[DBC2001]	(Dutra+Bica+Claria+, 2001)
Write:	<<[DBC2001] New Galaxy N>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Ref:	=2001A&A...371..895D
by	DUTRA C.M. , BICA E., CLARIA J.J., PIATTI A.E., AHUMADA A.V.
	Astron. Astrophys., 371, 895-907 (2001)
	Background galaxies as reddening probes throughout the Magellanic Clouds.
o	GH 90-060055-6840 = GH 10-4 in table 1.
o	Table 1, text: <[DBC2001] New Galaxy N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBC2004]
[DBC2004]	(De Breuck+Bertoldi+Carilli+, 2004)
Write:	<<[DBC2004] MNNa>> <<[DBC2004] R1>>
N:	10+3+1
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	MAMBO, VLA, and JCMT observations of the field around [DVR2000] TN J1338-1942: N=10 1.2mm sources are found. Use of VLT literature data. Three radio sources are found within a radius of 5 arcsec around the MAMBO source M2. R1 is only detected with the VLT and the VLA.
in source:	[DVR2000] TN J1338-1942
Ref:	=2004A&A...424....1D
by	DE BREUCK C. , BERTOLDI F., CARILLI C., OMONT A., VENEMANS B., ROETTGERING H., OVERZIER R., REULAND M., MILEY G., IVISON R., VAN BREUGEL W.
	Astron. Astrophys., 424, 1-12 (2004)
	A multi-wavelength study of the proto-cluster surrounding the z=4.1 radio galaxy TN J1338-1942.
o	Tables 1, 2, Fig.1: <[DBC2004] ANNa> (Nos M1-M10, M2a-M2c, R1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBC2016]
[DBC2016]	(Diego+Broadhurst+Chen+, 2016) (Not yet in Simbad)
Write:	<<[DBC2016] N.N>>
N:	21
Object:	LeG (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy)
Note:	N=21 gravitationally lensed images of galaxies located behind the galaxy cluster MCS J1149.5+2223. Use of HST ACS and WFC3 images, part of the HFF programme.
in source:	ClG J1149+2223 = MCS J1149.5+2223
Ref:	=2016MNRAS.456..356D
by	DIEGO J.M. , BROADHURST T., CHEN C., LIM J., ZITRIN A., CHAN B., COE D., FORD H.C., LAM D., ZHENG W.
	Mon. Not. R. Astron. Soc., 456, 356-365 (2016)
	A free-form prediction for the reappearance of supernova Refsdal in the Hubble Frontier Fields cluster MACSJ1149.5+2223.
o	Fig. 2: <[DBC2016] N.N> N=21 among( Nos 1.1-1.5 to 8.1-8.3).
o	P.362: MACS0516 is a probable misprint for MCS0416 (=MCS J0416.1-2403).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBC97]
[DBC97]	(Della Valle+Benetti+Cappellaro+, 1997)
Write:	<<[DBC97] Star A>> <<[DBC97] Star NN>>
N:	3+10
Object:	* (SIMBAD class: Star)
Note:	Stars in the field of Granat 1009-45. Maps. See also [SVC96], [FLM99].
Ref:	=1997A&A...318..179D
by	DELLA VALLE M. , BENETTI S., CAPPELLARO E., WHEELER C.
	Astron. Astrophys., 318, 179-186 (1997)
	The optical counterpart of GRS 1009-45 (X-ray Nova Velorum 1993).
o	Table 1: <[DBC97] Star A> (No. A), <[DBC97] Star NN> (Nos 1-10).
Ref:	=1999PASP..111..969F
by	FILIPPENKO A.V. , LEONARD D.C., MATHESON T., LI W., MORAN E.C., RIESS A.G.
	Publ. Astron. Soc. Pac., 111, 969-979 (1999)
	A black hole in the X-ray Nova Velorum 1993.
o	Fig.1: <[DBC97] Star A> (Nos B-C) added. Fig.9: <[FLM99] Star A> (Nos A-F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DBD
DBD	(DENIS Brown Dwarf) (Not yet in Simbad)
*****	Avoid the usage of DBD, prefer DENIS
Origin	of the Acronym: L (1998ApJ...509..836L)
Details on Acronym: [DBD86]
[DBD86]	(D'Odorico+Bandiera+Danziger+, 1986)
Write:	<<[DBD86] Star A>> <<[DBD86] Knot NN>>
N:	6+64
Object:	* + Em. knot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Deep image of the Kepler SNR: N=6 stars in the field. N= 64 emission knots in the SNR, see also vdBK, [BLV91].
in source:	NAME Kepler SNR
Ref:	=1986AJ.....91.1382D
by	D'ODORICO S. , BANDIERA R., DANZIGER J., FOCARDI P.
	Astron. J., 91, 1382-1385 (1986)
	A catalog of the H-α+NII emission features in the Kepler SNR.
o	in ref list DANZIGER 1980MNRAS.190p..47D instead of 1979
o	Table II: <[DBD86] Star A> (Nos A-F). Table III: <[DBD86] Knot NN> (Nos 1-64).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBE2005]
[DBE2005]	(Doherty+Bunker+Ellis+, 2005)
Write:	<<[DBE2005] CDFS NNNN>> <<[DBE2005] CDFS INNNN>> <<[DBE2005] NTT NNNN>> <<[DBE2005] SSA22 NNNN>>
N:	16+6+23+28
Object:	Extremely Red Obj. (SIMBAD class: Galaxy)
Note:	Keck LRIS and DEIMOS observations of EROs in 3 fields from Las Campanas Infrared Survey fields: CDFS, NTT, and SSA22 samples.
Ref:	=2005MNRAS.361..525D
by	DOHERTY M. , BUNKER A.J., ELLIS R.S., McCARTHY P.J.
	Mon. Not. R. Astron. Soc., 361, 525-549 (2005)
	The Las Campanas Infrared Survey - V. Keck spectroscopy of a large sample of extremely red objects.
o	ERO J164502+4626.4 = [HR94], MS 1054-03 = ClG 1054-03.
o	Table 2: <[DBE2005] CDFS NNNN> N=16 among (Nos 939-2158), <[DBE2005] CDFS INNNN> N=6 among (Nos I1843-I2163). Table 3: <[DBE2005] NTT NNNN> N=23 among (Nos 275-7463). Table 4: <[DBE2005] SSA22 NNNN> N=28 among (Nos 403-3378).
=E=	Catalogue in electronic form as J/MNRAS/361/525
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBE2008]
[DBE2008]	(Dominguez-Palmero+Balcells+Erwin+, 2008)
Write:	<<[DBE2008] NNNN>>
N:	248
Object:	G (SIMBAD class: Galaxy)
Note:	Spiral galaxies from archival HST WFPC2 and DEEP Groth Strip Survey data.
Ref:	=2008A&A...488.1167D
by	DOMINGUEZ-PALMERO L. , BALCELLS M., ERWIN P., PRIETO M., CRISTOBAL-HORNILLOS D., ELICHE-MORAL M.C., GUZMAN R.
	Astron. Astrophys., 488, 1167-1219 (2008)
	Bulges of disk galaxies at intermediate redshifts. I. Samples with and without bulges in the Groth Strip survey.
o	Tables a1, a2: <[DBE2008] NNNN> N=248 among (Nos 1-1142).
=E=	Catalogue in electronic form as J/A+A/488/1167
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBE2012]
[DBE2012]	(Deason+Belokurov+Evans+, 2012)= ([DBE2012a])
Write:	<<[DBE2012] FF-NN>>
N:	17
Object:	Poss. Blue HB* (SIMBAD class: HorBranch*_Candidate = Horizontal Branch Star Candidate)
Note:	VLT FORS2 spectroscopy of N=17 candidate member stars of the Hercules ultrafaint dwarf galaxy.
in source:	NAME Hercules Dwarf Galaxy
Ref:	=2012MNRAS.425L.101D
by	DEASON A.J. , BELOKUROV V., EVANS N.W., WATKINS L.L., FELLHAUER M.
	Mon. Not. R. Astron. Soc., 425L, 101-105 (2012)
	The stretching of Hercules.
o	Table 2: <[DBE2012] FF-NN> N=17 among (Nos F1-09 to F1-21, F2-01 to F2-20, F3-02 to F3-07).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBE2012a]
[DBE2012a]	(Deason+Belokurov+Evans+, 2012) (Not yet in Simbad)
*****	Avoid the usage of [DBE2012a], prefer [DBE2012]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBE2012b]
[DBE2012b]	(Deason+Belokurov+Evans+, 2012)
Write:	<<[DBE2012b] 85-TARGNN>> <<[DBE2012b] 88-TARGNNN>>
N:	38
Object:	Blue * (SIMBAD class: Star)
Note:	VLT FORS2 spectroscopy of N=38 candidate blue horizontal branch (BHB) stars in the SDSS Stripe 82.
Ref:	=2012MNRAS.425.2840D
by	DEASON A.J. , BELOKUROV V., EVANS N.W., KOPOSOV S.E., COOKE R.J., PENARRUBIA J., LAPORTE C.F.P., FELLHAUER M., WALKER M.G., OLSZEWSKI E.W.
	Mon. Not. R. Astron. Soc., 425, 2840-2853 (2012)
	The cold veil of the Milky way stellar halo.
o	Table 1: <[DBE2012b] 8N-TARGNNN> N=38 among (85-TARG2 to 85-TARG38 and 88-TARG2 to 88-TARG110).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBG2009]
[DBG2009]	(DeRose+Bourke+Gutermuth+, 2009)
Write:	<<[DBG2009] NNN>>
N:	483
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	VLT NACO AO-assisted NIR observations of RCW 38.
in source:	RCW 38
Ref:	=2009AJ....138...33D
by	DEROSE K.L. , BOURKE T.L., GUTERMUTH R.A., WOLK S.J., MEGEATH S.T., ALVES J., NURNBERGER D.
	Astron. J., 138, 33-45 (2009)
	A Very Large Telescope/NACO study of star formation in the massive embedded cluster RCW 38.
o	Table 1: <[DBG2009] NNN> (Nos 1-483).
=E=	Catalogue in electronic form as J/AJ/138/33
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBG2011]
[DBG2011]	(Davies+Bastian+Gieles+, 2011)
Write:	<<[DBG2011] NN>>
N:	55
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT ISAAC spectroscopy of the stellar cluster GLIMPSE C01.
in source:	GLIMPSE C01
Ref:	=2011MNRAS.411.1386D
by	DAVIES B. , BASTIAN N., GIELES M., SETH A.C., MENGEL S., KONSTANTOPOULOS I.S.
	Mon. Not. R. Astron. Soc., 411, 1386-1394 (2011)
	GLIMPSE-CO1: the most massive intermediate-age stellar cluster in the galaxy.
o	Table 1: <[DBG2011] NN> (Nos 1-55).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBG99]
[DBG99]	(De Grandi+Bohringer+Guzzo+, 1999)
Write:	<<[DBG99] NNN>>
N:	130
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	ROSAT All-Sky Survey (RASS1) analysis.
Ref:	=1999ApJ...514..148D
by	DE GRANDI S. , BOHRINGER H., GUZZO L., MOLENDI S., CHINCARINI G., COLLINS C., CRUDDACE R., NEUMANN D., SCHINDLER S., SCHUECKER P., VOGES W.
	Astrophys. J., 514, 148-163 (1999)
	A flux-limited sample of bright clusters of galaxies from the southern part of the ROSAT all-sky survey: the catalog and log n-log s.
o	(Erratum) Erratum vol. 528, p. 1035 (2000)
o	Table 1: <[DBG99] NNN> (Nos 1-130).
=E=	Catalogue in electronic form as J/ApJ/514/148
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBI2015]
[DBI2015]	(Dirienzo+Brogan+Indebetouw+, 2015)
Write:	<<[DBI2015] JHHMMSS+DDMMSS>>
N:	81
Object:	Clump (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	GBT and VLA NH3 and CCS line observations of N=81 millimeter continuum clumps in nine Infrared Dark Clouds (IRDCs). Use of Spitzer MIPSGAL and Herschel data.
Ref:	=2015AJ....150..159D
by	DIRIENZO W.J. , BROGAN C., INDEBETOUW R., CHANDLER C.J., FRIESEN R.K., DEVINE K.E.
	Astron. J., 150, 159 (2015)
	Physical conditions of the earliest phases of massive star formation: single-dish and interferometric observations of ammonia and CCS in infrared dark clouds.
o	G028.83-00.19 is a probable misprint for G028.23-00.19.
o	Table 5: <[DBI2015] JHHMMSS+DDMMSS> N=81.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBK2009]
[DBK2009]	(Dobashi+Bernard+Kawamura+, 2009)
Write:	<<[DBK2009] A>>
N:	10
Object:	Dark Cloud (SIMBAD class: DarkNeb = Dark Cloud (nebula))
Stat:	is completely incorporated in Simbad
Note:	Dark clouds in the Small Magellanic Cloud based on the SIRIUS and 6X 2MASS point source catalogs.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2009AJ....137.5099D
by	DOBASHI K. , BERNARD J.-P., KAWAMURA A., EGUSA F., HUGHES A., PARADIS D., BOT C., REACH W.T.
	Astron. J., 137, 5099-5109 (2009)
	Extinction map of the Small Magellanic Cloud based on the SIRIUS and 6X 2MASS point source catalogs.
o	Table 1: <[DBK2009] A> (Nos A-J).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBK2016]
[DBK2016]	(Dieball +bedin+Knigge+, 2016)
Write:	<<[DBK2016] BDN>> <<[DBK2016] WDN>>
N:	4+4
Object:	Poss. Brown Dwarf + WD (SIMBAD class: Star)
Note:	HST WFC3 photometric NIR observations of N=4+4 brown dwarf candidates and white dwarfs in the globular cluster M4. Use of archival HST optical data/
in source:	M 4 = NGC 6121
Ref:	=2016ApJ...817...48D
by	DIEBALL A. , BEDIN L.R., KNIGGE C., RICH R.M., ALLARD F., DOTTER A., RICHER H., ZUREK D.
	Astrophys. J., 817, 48 (2016)
	Deep Near-IR observations of the globular cluster M4: hunting for brown dwarfs.
o	Table 2: <[DBK2016] BDN> (Nos 1-4). Table 3: <[DBK2016] WDN> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBL2003]
[DBL2003]	(Demers+Battinelli+Letarte, 2003)= ([DBL2003a])
Write:	<<[DBL2003] NNN>>
N:	532
Object:	C* (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Note:	CFH12K observations. See also [GGR2006] in NGC 205. See also [ADK2000], [BD2000], [DB2002], [LDB2002], [BDL2003], [DBL2003b], [BD2004a], [BD2004b], [DBL2004].
in source:	NGC 205 = M 110
Ref:	=2003AJ....125.3037D
by	DEMERS S. , BATTINELLI P., LETARTE B.
	Astron. J., 125, 3037-3045 (2003)
	Carbon star survey in the Local Group. VI. The dwarf spheroidal galaxy NGC 205.
o	Table 1: <[DBL2003] NNN> (Nos 1-532).
=E=	Catalogue in electronic form as J/AJ/125/3037
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBL2003a]
[DBL2003a]	(Demers+Battinelli+Letarte, 2003)
*****	Avoid the usage of [DBL2003a], prefer [DBL2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBL2003b]
[DBL2003b]	(Demers+Battinelli+Letarte, 2003)
Write:	<<[DBL2003b] NNN>>
N:	446
Object:	C* (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Note:	CFHT observations. See also [ADK2000], [BD2000], [DB2002], [BDL2003], [DBL2003], [DBL2003b], [BD2004a], [BD2004b], [DBL2004].
in source:	NGC 3109
Ref:	=2003A&A...410..795D
by	DEMERS S. , BATTINELLI P., LETARTE B.
	Astron. Astrophys., 410, 795-801 (2003)
	Carbon star survey in the Local Group. VII. NGC 3109 a galaxy without a stellar halo.
o	Table 2: <[DBL2003b] NNN> (Nos 1-446).
=E=	Catalogue in electronic form as J/A+A/410/795
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBL2004]
[DBL2004]	(Demers+Battinelli+Letarte, 2004)
Write:	<<[DBL2004] NNN>>
N:	676
Object:	C* (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Note:	Carbon stars in IC 10 from CFHT observations using the CFH12K camera.
in source:	IC 10
Ref:	=2004A&A...424..125D
by	DEMERS S. , BATTINELLI P., LETARTE B.
	Astron. Astrophys., 424, 125-132 (2004)
	A Carbon star approach to IC 10: Distance and correct size.
o	Table 2: <[DBL2004] NNN> (Nos 1-676).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBL2010]
[DBL2010]	(Dopita+Blair+Long+, 2010)
Write:	<<[DBL2010] M83-SNR-1-NN>> <<[DBL2010] M83-SNR-N-NN>> <<[DBL2010] M83-SRC-1-ON>>
N:	40+19+5
Object:	Poss. SNR + [OIII] source (SIMBAD class: EmObj = Emission Object)
Stat:	is completely incorporated in Simbad
Note:	HST WFC3 observations of N∼60 SNR candidates and N=5 young ejecta-dominated candidates in M83.
in source:	NGC 5236 = M 83
Ref:	=2010ApJ...710..964D
by	DOPITA M.A. , BLAIR W.P., LONG K.S., MUTCHLER M., WHITMORE B.C., KUNTZ K.D., BALICK B., BOND H.E., CALZETTI D., CAROLLO M., DISNEY M., FROGEL J.A., O'CONNELL R., HALL D., HOLTZMAN J.A., KIMBLE R.A., MacKENTY J., McCARTHY P., PARESCE F., SAHA A., SILK J., SIRIANNI M., TRAUGER J., WALKER A.R., WINDHORST R., YOUNG E.
	Astrophys. J., 710, 964-978 (2010)
	Supernova remnants and the interstellar medium of M83: imaging and photometry with the wide field camera 3 on the Hubble space telescope.
o	Table 2: <[DBL2010] M83-SNR-1-NN> (Nos 1-40). Table 3: <[DBL2010] M83-SNR-N-NN> (Nos N-01 to N-19). Table 4: <[DBL2010] M83-SRC-1-ON> (Nos O1-O5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBL2011]
[DBL2011]	(Dhital+Burgasser+Looper+, 2011)
Write:	<<[DBL2011] 2MASS J0130-4445>> <<[DBL2011] 2MASS J0130-4445A>>
N:	1+2
Object:	** + LM* (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	IRTF SpeX spectroscopic observations of 2MASS J01303563-4445411.
Ref:	=2011AJ....141....7D
by	DHITAL S. , BURGASSER A.J., LOOPER D.L., STASSUN K.G.
	Astron. J., 141, 7 (2011)
	Resolved spectroscopy of M Dwarf/L dwarf binaries. IV. Discovery of AN M9 + L6 binary separated by over 100 AU.
o	<[DBL2011] 2MASS J0130-4445> N=1, <[DBL2011] 2MASS J0130-4445A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBL2017]
[DBL2017]	(Diehl+Buckley-Geer+Lindgren+, 2017)
Write:	<<[DBL2017] DES JHHMM+DDMM>> <<[DBL2017] DES JHHMM+DDMMA>> <<[DBL2017] DES JHHMM+DDMM (A)>> <<[DBL2017] DES JHHMM+DDMM (N)>>
N:	616+10+679+1072
Object:	Poss. Grav. lens system + Poss. Grav. lens + Poss. Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=679 gravitational lens candidates and N=1072 gravitationally lensed image candidates in 616+10 strong gravitational lens candidate systems. Use of data from the Dark Energy Survey (DES) Science Verification and Year 1 observations (cf. 2017ApJS..232...15D), and from the combined results of eight searches in the full 5000 square degrees of DES osbervations.
Ref:	=2017ApJS..232...15D
by	DIEHL H.T. , BUCKLEY-GEER E.J., LINDGREN K.A., NORD B., GAITSCH H., GAITSCH S., LIN H., ALLAM S., COLLETT T.E., FURLANETTO C., GILL M.S.S., MORE A., NIGHTINGALE J., ODDEN C., PELLICO A., TUCKER D.L., DA COSTA L.N., NETO A.F., KUROPATKIN N., SOARES-SANTOS M., WELCH B., ZHANG Y., FRIEMAN J.A., ABDALLA F.B., ANNIS J., BENOIT-LEVY A., BERTIN E., BROOKS D., BURKE D.L., CARNERO ROSELL A., CARRASCO KIND M., CARRETERO J., CUNHA C.E., D'ANDREA C.B., DESAI S., DIETRICH J.P., DRLICA-WAGNER A., EVRARD A.E., FINLEY D.A., FLAUGHER B., GARCIA-BELLIDO J., GERDES D.W., GOLDSTEIN D.A., GRUEN D., GRUENDL R.A., GSCHWEND J., GUTIERREZ G., JAMES D.J., KUEHN K., KUHLMANN S., LAHAV O., LI T.S., LIMA M., MAIA M.A.G., MARSHALL J.L., MENANTEAU F., MIQUEL R., NICHOL R.C., NUGENT P., OGANDO R.L.C., PLAZAS A.A., REIL K., ROMER A.K., SAKO M., SANCHEZ E., SANTIAGO B., SCARPINE V., SCHINDLER R., SCHUBNELL M., SEVILLA-NOARBE I., SHELDON E., SMITH M., SOBREIRA F., SUCHYTA E., SWANSON M.E.C., TARLE G., THOMAS D., WALKER A.R., (The DES Collaboration)
	Astrophys. J., Suppl. Ser., 232, 15-15 (2017)
	The DES Bright Arcs Survey: hundreds of candidate strongly lensed galaxy systems from the Dark Energy Survey Science Verification and Year 1 observations.
o	Table 3: <[DBL2017] DES JHHMM+DDMM> N=374, <[DBL2017] DES JHHMM+DDMM (A)>, <[DBL2017] DES JHHMM+DDMM (N)>, N=1091.
Ref:	=2022ApJS..259...27O
by	O'DONNELL J.H. , WILKINSON R.D., DIEHL H.T., AROS-BUNSTER C., BECHTOL K., BIRRER S., BUCKLEY-GEER E.J., CARNERO ROSELL A., CARRASCO KIND M., DA COSTA L.N., GONZALEZ LOZANO S.J., GRUENDL R.A., HILTON M., LIN H., LINDGREN K.A., MARTIN J., PIERES A., RYKOFF E.S., SEVILLA-NOARBE I., SHELDON E., SIFON C., TUCKER D.L., YANNY B., ABBOTT T.M.C., AGUENA M., ALLAM S., ANDRADE-OLIVEIRA F., ANNIS J., BERTIN E., BROOKS D., BURKE D.L., CARRETERO J., COSTANZI M., DE VICENTE J., DESAI S., DIETRICH J.P., ECKERT K., EVERETT S., FERRERO I., FLAUGHER B., FOSALBA P., FRIEMAN J., GARCIA-BELLIDO J., GAZTANAGA E., GERDES D.W., GRUEN D., GSCHWEND J., GILL M.S.S., GUTIERREZ G., HINTON S.R., HOLLOWOOD D.L., HONSCHEID K., JAMES D.J., JELTEMA T., KUEHN K., LAHAV O., LIMA M., MAIA M.A.G., MARSHALL J.L., MELCHIOR P., MENANTEAU F., MIQUEL R., MORGAN R., NORD B., OGANDO R.L.C., PAZ-CHINCHON F., PEREIRA M.E.S., PLAZAS MALAGON A.A., RODRIGUEZ-MONROY M., ROMER A.K., ROODMAN A., SANCHEZ E., SCARPINE V., SCHUBNELL M., SERRANO S., SMITH M., SUCHYTA E., SWANSON M.E.C., TARLE G., THOMAS D., TO C., VARGA T.N., (The DES Collaboration)
	Astrophys. J., Suppl. Ser., 259, 27-27 (2022)
	The Dark Energy Survey Bright Arcs Survey: Candidate Strongly Lensed Galaxy Systems from the Dark Energy Survey 5000 Square Degree Footprint.
o	Table 3: <[DBL2017] DES JHHMM+DDMM> N=242, <[DBL2017] DES JHHMM+DDMMA> N=10. Figs 10-17, Table 4: <[DBL2017] DES JHHMM+DDMMA (A)> N=262, <[DBL2017] DES JHHMM+DDMMA (N)> N=398.
=E=	Catalogue in electronic form as <J/ApJS/232/15/>
=E=	Catalogue in electronic form as <J/ApJS/259/27/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBM2003]
[DBM2003]	(Della Valle+Benetti+Malesani+, 2003)
Write:	<<[DBM2003] nearby G>> <<[DBM2003] host G>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Search for the host galaxy of GRB 021211: authors confirm a nearby galaxy at z=0.80 and the host galaxy at z=1.004.
Ref:	=2003GCN..1809....1D
by	DELLA VALLE M. , BENETTI S., MALESANI D., MASON E., ANTONELLI L.A., COCOZZA G., COVINO S., FUGAZZA D., GHISELLINI G., ISRAEL G.L., STELLA L., TESTA V.
	GRB Coordinates Network, Circular Service, 1809, 1-None (2003)
	GRB 021211: VLT spectrum.
o	<[DBM2003] nearby G> N=1, <[DBM2003] host G> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBM2004]
[DBM2004]	(Drake+Bicknell+McGregor+, 2004)
Write:	<<[DBM2004] IRAS FHHMMm+DDMM A>>
N:	21
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA, LBA, and VLA observations of FIR-luminous radio-excess galaxies.
in source:	IRAS F01477-1655
in source:	IRAS F03265-2852
in source:	IRAS F04367-2726
in source:	IRAS F08064-1018
in source:	IRAS F19254-7245
in source:	IRAS F20203-5733
in source:	IRAS F23075-5957
in source:	IRAS F10418+1153
Ref:	=2004AJ....128..969D
by	DRAKE C.L. , BICKNELL G.V., McGREGOR P.J., DOPITA M.A.
	Astron. J., 128, 969-984 (2004)
	Radio-excess IRAS galaxies. III. Radio properties.
o	Tables 1, 2: <[DBM2004] IRAS FHHMMm+DDMM A> N=21.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBM2007]
[DBM2007]	(DeGraaff+Blakeslee+Meurer+, 2007)
Write:	<<[DBM2007] NNNN>>
N:	151
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	HST ACS HRC observations of NGC 1533.
in source:	NGC 1533
Ref:	=2007ApJ...671.1624D
by	DEGRAAFF R.B. , BLAKESLEE J.P., MEURER G.R., PUTMAN M.E.
	Astrophys. J., 671, 1624-1639 (2007)
	A galaxy in transition: structure, globular clusters, and distance of the star-forming S0 galaxy NGC 1533 in Dorado.
o	Table 2: <[DBM2007] NNNN> N=151 among (Nos 13-7509).
=E=	Catalogue in electronic form as J/ApJ/671/1624
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBM2010]
[DBM2010]	(Davidge+Beck+McGregor, 2010) (Not yet in Simbad)
Write:	<<[DBM2010] NN>>
N:	14
Object:	* (SIMBAD class: Star)
Note:	Gemini North NFIS+ALTAIR observations of the center of M32.
in source:	M 32
Ref:	=2010PASP..122..241D
by	DAVIDGE T.J. , BECK T.L., McGREGOR P.J.
	PASP, 122, 241-247 (2010)
	Identifying bright stars in crowded environments using velocity dispersion measurements, and an application to the center of M32.
o	Fig. 1, Table 1: <[DBM2010] NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBM2014]
[DBM2014]	(Downes+Briceno+Mateu+, 2014)
Write:	<<[DBM2014] NNNN>> <<[DBM2014] DDD.ddd+DD.ddd>>
N:	75+17
Object:	Star (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	MMT Hectospec observations of N=77 low-mass stars and N=17 stars showing transitional or evolved disks in the 25 Orionis Group.
in source:	NAME 25 ORI GROUP
Ref:	=2014MNRAS.444.1793D
by	DOWNES J.J. , BRICENO C., MATEU C., HERNANDEZ J., VIVAS A.K., CALVET N., HARTMANN L., PETR-GOTZENS M.G., ALLEN L.
	Mon. Not. R. Astron. Soc., 444, 1793-1811 (2014)
	The low-mass star and sub-stellar populations of the 25 Orionis group.
o	Tables 4-5: <[DBM2014] NNNN> N=75 among (Nos 1232-1400). Table 8: <[DBM2014] DDD.ddd+DD.ddd> N=17.
=E=	Catalogue in electronic form as <J/MNRAS/444/1793/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBM95]
[DBM95]	(Davis+Bird+Mushotzky+, 1995)
Write:	<<[DBM95] SN>> <<[DBM95] Clump A>>
N:	3+3
Object:	(X) + Clump (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Tables 2, 3: extended X sources, (Nos 1-3) Table 4: Clump (Nos A-C)
in source:	ACO 548
Ref:	=1995ApJ...440...48D
by	DAVIS D.S. , BIRD C.M., MUSHOTZKY R.F., ODEWAHN S.C.
	Astrophys. J., 440, 48-59 (1995)
	Abell 548 : an X-ray and optical analysis of substructure.
o	Tables 2, 3: <[DBM95] SN> N=3, Table4: <[DBM95] Clump A> N=3
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBO2016]
[DBO2016]	(Dewangan+Baug+Ojha+, 2016)
Write:	<<[DBO2016] N46clm>> <<[DBO2016] clmN>> <<[DBO2016] CRSNN>>
N:	1+3+10
Object:	Molecular Condensation + Compact Radio Source (SIMBAD class: Unknown = Object of Unknown Nature)
Stat.	in SIMBAD: Table 3 is not in Simbad.
Note:	Himalayan Chandra 2m telescope (HCT, India) HFOSC and TIRSPEC observations of N=1+3 molecular condensations. N=20 compact radio sources extracted from VLA MAGPIS data.
in source:	[CPA2006] N46
Ref:	=2016ApJ...826...27D
by	DEWANGAN L.K. , BAUG T., OJHA D.K., JANARDHAN P., NINAN J.P., LUNA A., ZINCHENKO I.
	Astrophys. J., 826, 27-27 (2016)
	Star-formation activity in the neighborhood of W-R 1503-160L star in the mid-infrared bubble N46.
o	Table 3: sources CRS1-CRS10 are not in SIMBAD.
o	Fig. 3, Table 2: <[DBO2016] N46clm> N=1, <[DBO2016] clmN> (Nos clm1-clm3). Fig. 4, Table 3: <[DBO2016] CRSNN> (Nos CRS1-CRS10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBO2018]
[DBO2018]	(Dewangan+Baug+Ojha+, 2018) (Not yet in Simbad)
Write:	<<[DBO2018] IRcmmeN>> <<[DBO2018] sN>> <<[DBO2018] nN>>
N:	2+8+5
Object:	Clump + (Rad) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT NAOS-CONICA observations of N=2 sources in IRAS 17008-4040 I. GMRT 0.61 and 1.28 GHz radio continuum maps of N=8+5 ionized clumps in IRAS 17008-4040 and IRAS 17009-4042. Use of archival data from several surveys: GMRT, ThrUMMS, ATLASGAL, Hi-GAL, Spitzer GLIMPSE, VLT NAOS-CONICA, VVV, 2MASS.
in source:	IRAS 17008-4040
in source:	IRAS 17009-4042
Ref:	=2018ApJ...869...30D
by	DEWANGAN L.K. , BAUG T., OJHA D.K., GHOSH S.K.
	Astrophys. J., 869, 30-30 (2018)
	Investigating inner and large-scale physical environments of IRAS 17008-4040 and IRAS 17009-4042 toward L' = 345°.5, b = 0°.3.
o	Texte: <[DBO2018] IRcmmeN> (Nos 1 to 2). Table 3: <[DBO2018] sN> (Nos 1 to 8), <[DBO2018] nN> (Nos 1 to 5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBP2006]
[DBP2006]	(De Wit+Bouvier+Palla+, 2006)= (IC4665)
Write:	<<[DBP2006] JHHMMSS.ss+DDMMSS.s>>
N:	785
Object:	* in Cl* (SIMBAD class: Star)
Note:	CFH12K camera observations of IC 4665.
in source:	IC 4665
Ref:	=2006A&A...448..189D
by	DE WIT W.J. , BOUVIER J., PALLA F., CUILLANDRE J.-C., JAMES D.J., KENDALL T.R., LODIEU N., McCAUGHREAN M.J., MORAUX E., RANDICH S., TESTI L.
	Astron. Astrophys., 448, 189-202 (2006)
	Exploring the lower mass function in the young open cluster IC 4665.
o	Table 3: <[DBP2006] JHHMMSS.ss+DDMMSS.s> (Nos 1-785).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBP2019]
[DBP2019]	(de La Vieuville+Bina+Pello+, 2019)
Write:	<<[DBP2019] ANNNN NNN>> <<[DBP2019] A2390 L1>>
N:	11+1
Object:	Lensed LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT MUSE observations of N=11+1 Lyman-alpha emitters (LAEs), lensed by galaxy clusters ACO 2390 and ACO 2667. See also [BPR2016] (in ACO 1689) and [MRC2018] (in ACO 2744).
in source:	ACO 2390
in source:	ACO 2667
Ref:	=2019A&A...628A...3D
by	DE LA VIEUVILLE G. , BINA D., PELLO R., MAHLER G., RICHARD J., DRAKE A.B., HERENZ E.C., BAUER F.E., CLEMENT B., LAGATTUTA D., LAPORTE N., MARTINEZ J., PATRICIO V., WISOTZKI L., ZABL J., BOUWENS R.J., CONTINI T., GAREL T., GUIDERDONI B., MARINO R.A., MASEDA M.V., MATTHEE J., SCHAYE J., SOUCAIL G.
	Astron. Astrophys., 628A, 3-3 (2019)
	Faint end of the z ~ 3-7 luminosity function of Lyman-α emitters behind lensing clusters observed with MUSE.
o	Table E.1: <[DBP2019] ANNNN NNN> N=11 among (Nos A2390 71-A2390 243, A2667 24-A2667 62), <[DBP2019] A2390 L1> N=1.
=E=	Catalogue in electronic form as <J/A+A/628/A3/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBR2015]
[DBR2015]	(Drlica-Wagner+Bechtol+Rykoff+, 2015)
Write:	<<[DBR2015] DES JHHMM+DDMM>>
N:	8
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=8 ultra-faint dwarf galaxy candidates, using optical imaging data collected during the second year of the Dark Energy Survey (DES).
Ref:	=2015ApJ...813..109D
by	DRLICA-WAGNER A. , BECHTOL K., RYKOFF E.S., LUQUE E., QUEIROZ A., MAO Y.-Y., WECHSLER R.H., SIMON J.D., SANTIAGO B., YANNY B., BALBINOT E., DODELSON S., NETO A.F., JAMES D.J., LI T.S., MAIA M.A.G., MARSHALL J.L., PIERES A., STRINGER K., WALKER A.R., ABBOTT T.M.C., ABDALLA F.B., ALLAM S., BENOIT-LEVY A., BERNSTEIN G.M., BERTIN E., BROOKS D., BUCKLEY-GEER E., BURKE D.L., CARNERO ROSELL A., CARRASCO KIND M., CARRETERO J., CROCCE M., DA COSTA L.N., DESAI S., DIEHL H.T., DIETRICH J.P., DOEL P., EIFLER T.F., EVRARD A.E., FINLEY D.A., FLAUGHER B., FOSALBA P., FRIEMAN J., GAZTANAGA E., GERDES D.W., GRUEN D., GRUENDL R.A., GUTIERREZ G., HONSCHEID K., KUEHN K., KUROPATKIN N., LAHAV O., MARTINI P., MIQUEL R., NORD B., OGANDO R., PLAZAS A.A., REIL K., ROODMAN A., SAKO M., SANCHEZ E., SCARPINE V., SCHUBNELL M., SEVILLA-NOARBE I., SMITH R.C., SOARES-SANTOS M., SOBREIRA F., SUCHYTA E., SWANSON M.E.C., TARLE G., TUCKER D., VIKRAM V., WESTER W., ZHANG Y., ZUNTZ J., (The DES Collaboration)
	Astrophys. J., 813, 109 (2015)
	Eight ultra-faint galaxy candidates discovered in year two of the dark energy survey.
o	Tables 1-2: <[DBR2015] DES JHHMM+DDMM> N=8. <NAME Grus II> = <NAME Gru II>. <NAME Tucana R > = <NAME Tuc R> (Nos III-V) added. <NAME Columba I> = <NAME Col I>. <NAME Reticulum III> = <NAME Ret III>. <NAME Indus II> = <NAME Ind II>. <NAME Cetus II> = <NAME Cet II>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBR99]
[DBR99]	(Devine+Bally+Reipurth+, 1999)
Write:	<<[DBR99] G192.16>> <<[DBR99] UK N>>
N:	1+4
Object:	YSO + Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Discovery of N=1 YSO 'G192.16' associated with the HII region 'GAL 192.16-03.82'. East of G192.16 HH 396 and HH 397 and 4 associated features UK 1 to UK 4.
Ref:	=1999AJ....117.2919D
by	DEVINE D. , BALLY J., REIPURTH B., SHEPHERD D., WATSON A.
	Astron. J., 117, 2919-2930 (1999)
	A giant Herbig-Haro flow from a massive young star in G192.16-3.82.
o	Knots of 'HH NNN' objects are 'HH NNNA' in SIMBAD.
o	<HH NNN> (Nos 396-397). Table 1: <[DBR99] G192.16> = <NAME G 192.16> N=1, <[DBR99] UK N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DBS
DBS	(D'Odorico+Benvenuti+Sabbadin)= (D)
Write:	<<DBS N>>
N:	3+2
Object:	SNR + Poss. SNR (SIMBAD class: SNRemnant = SuperNova Remnant)
Stat:	is completely incorporated in Simbad
Note:	Identif. charts
in source:	M 33 = NGC 598
Ref:	=1978A&A....63...63D
by	D'ODORICO S. , BENVENUTI P., SABBADIN F.
	Astron. Astrophys., 63, 63-68 (1978)
	Supernova remnants in M 33.
o	:<DBS N> (Nos 1-5).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [DBS2000]
[DBS2000]	(Duc+Brinks+Springel+, 2000)= (TDG)
Write:	<<[DBS2000] TDG N>> <<[DBS2000] JHHMMSS.ss+DDMMSS.s>>
N:	5+2
Object:	G + Part of G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 6, Fig.16: N=5 condensations in the 'TDG' (Tidal Dwarf Galaxy) [BLD2000] APG 245N. Text: N=2 uncataloged background galaxies.
in source:	APG 245
Ref:	=2000AJ....120.1238D
by	DUC P.-A. , BRINKS E., SPRINGEL V., PICHARDO B., WEILBACHER P., MIRABEL I.F.
	Astron. J., 120, 1238-1264 (2000)
	Formation of a tidal dwarf galaxy in the interacting system Arp 245 (NGC 2992/93).
o	Par. 2.4 : calibrator 1331+305 = RORF 1328+307, calibrator 0902-142 = R ORF 0859-140.
o	Table 6, Fig.16: <[DBS2000] TDG N> (Nos 1-5). Text: <[DBS2000] JHHMMSS.ss+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBS2003]
[DBS2003]	(Dutra+Bica+Soares+, 2003)= (DBSB)
Write:	<<[DBS2003] NNN>>
N:	179
Object:	IR-Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	2MASS survey of infrared stellar clusters in the Milky Way. See also Paper II [BDS2003].
Ref:	=2003A&A...400..533D
by	DUTRA C.M. , BICA E., SOARES J., BARBUY B.
	Astron. Astrophys., 400, 533-539 (2003)
	New infrared star clusters in the southern Milky Way with 2MASS.
o	Table 2 : Stk 16 = Cl Stock 16. Fig.7 : GG 2 = [GG70] An 2.
o	Tables 3, 4: <[DBS2003] NNN> (Nos 1-179).
=E=	Catalogue in electronic form as J/A+A/400/533
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBS2005]
[DBS2005]	(Dey+Bian+Soifer+, 2005)= (SST24)
Write:	<<[DBS2005] SST24 JHHMMSS.s+DDMMSS>> <<[DBS2005] Galaxy A>> <<[DBS2005] JHHMMSS.s+DDMMSS>> (not recognised by Simbad, but found in literature)
N:	1+2
Object:	Nebula + G + (IR) (SIMBAD class: ISM = Interstellar Medium Object)
Stat:	is completely incorporated in Simbad
Note:	Spitzer MIPS 24 mu.m (SST24) and Keck LRIS observations at 24mu.m (SST24): discovery of a Ly-alpha emitting nebula which comprises a MIPS source and a galaxy (A). An other galaxy B is probably a background galaxy.
Ref:	=2005ApJ...629..654D
by	DEY A. , BIAN C., SOIFER B.T., BRAND K., BROWN M.J.I., CHAFFEE F.H., LE FLOC'H E., HILL G., HOUCK J.R., JANNUZI B.T., RIEKE M., WEEDMAN D., BRODWIN M., EISENHARDT P.
	Astrophys. J., 629, 654-666 (2005)
	Discovery of a large ~200 kpc gaseous nebula at z ~ 2.7 with the Spitzer Space Telescope.
o	<[DBS2005] SST24 JHHMMSS.s+DDMMSS> N=1. <[DBS2005] Galaxy A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBS2007]
[DBS2007]	(Douglas+Bremer+Stanway+, 2007)
Write:	<<[DBS2007] JHHMMSS.s+DDMMSS.s>>
N:	1
Object:	AGN (SIMBAD class: AGN = Active Galaxy Nucleus)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 and NTT SOFI observations: discovery of a faint AGN.
Ref:	=2007MNRAS.376.1393D
by	DOUGLAS L.S. , BREMER M.N., STANWAY E.R., LEHNERT M.D.
	Mon. Not. R. Astron. Soc., 376, 1393-1398 (2007)
	Discovery of a single faint AGN in a large sample of z > 5 Lyman break galaxies.
o	<[DBS2007] JHHMMSS.s+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBS2010]
[DBS2010]	(Davies+Bremer+Stanway+, 2010)
Write:	<<[DBS2010] DDD.ddd+DD.dddd>>
N:	8
Object:	LBG (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ATCA observations of one field (J1054.4-1245) of the ESO Remote Galaxy Survey.
Ref:	=2010MNRAS.408L..31D
by	DAVIES L.J.M. , BREMER M.N., STANWAY E.R., BIRKINSHAW M., LEHNERT M.D.
	Mon. Not. R. Astron. Soc., 408L, 31-35 (2010)
	Limits on the molecular gas content of z ~ 5 LBGs.
o	Table 1: <[DBS2010] DDD.ddd+DD.dddd> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBS2012]
[DBS2012]	(De Buizer+Bartkiewicz+Szymczak, 2012)
Write:	<<[DBS2012] GLL.lll+BB.bbb:BDS12N>>
N:	15 (SIMBAD class: Infrared = Infra-Red Source)
Note:	Gemini South T-ReCS MIR and Gemini North NIRI observations of massive young stellar objects with ring-like distributions of maser spots.
Ref:	=2012ApJ...754..149D
by	DE BUIZER J.M. , BARTKIEWICZ A., SZYMCZAK M.
	Astrophys. J., 754, 149 (2012)
	Testing the hypothesis that methanol maser rings trace circumstellar disks: high-resolution near-infrared and mid-infrared imaging.
o	Table 1: <[DBS2012] {G}LL.lll+BB.bbb{:BDS12}N> N=15
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBS2015]
[DBS2015]	(Dias+Barbuy+Saviane +, 2015)
Write:	<<[DBS2015] NGCNNNN NN>> <<[DBS2015] M71 NN>> <<[DBS2015] Terzan8 NN>>
N:	86 (SIMBAD class: RGB* = Red Giant Branch star)
Note:	VLT FORS2 observations of N=86 red giant stars in the globular clusters NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426 and in Terzan 8.
in source:	NGC 6528
in source:	NGC 6553
in source:	M 71 = NGC 6836
in source:	NGC 6558
in source:	NGC 6426
in source:	Cl Terzan 8
Ref:	=2015A&A...573A..13D
by	DIAS B. , BARBUY B., SAVIANE I., HELD E.V., DA COSTA G.S., ORTOLANI S., VASQUEZ S., GULLIEUSZIK M., KATZ D.
	Astron. Astrophys., 573A, 13-13 (2015)
	FORS2/VLT survey of Milky Way globular clusters. I. Description of the method for derivation of metal abundances in the optical and application to NGC 6528, NGC 6553, M 71, NGC 6558, NGC 6426, and Terzan 8.
o	Tables 3, 6: <[DBS2015] NGCNNNN NN>, <[DBS2015] M71 NN>, <[DBS2015] TerzanN NN>, N=86.
=E=	Catalogue in electronic form as <J/A+A/573/A13/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DBSB
DBSB	(Dutra+Bica+Soares+Barbuy)
*****	Avoid the usage of DBSB, prefer [DBS2003]
Origin	of the Acronym: L (2008A&A...478..419S)
Details on Acronym: [DBT2008]
[DBT2008]	(Dowell+Buckalew+Tan, 2008)
Write:	<<[DBT2008] NGC NNNN NNNN>> <<[DBT2008] IC 3521 N>> <<[DBT2008] UGC NNNN NN>> <<[DBT2008] DDO NNN NN>>
N:	933
Object:	Super Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Search for Super Star Clusters in N=16 galaxies from SDSS DR5 data.
Ref:	=2008AJ....135..823D
by	DOWELL J.D. , BUCKALEW B.A., TAN J.C.
	Astron. J., 135, 823-835 (2008)
	The initial cluster mass function of super star clusters in irregular and spiral galaxies.
o	Table 2: <[DBT2008] NGC NNNN NNNN>, <[DBT2008] IC 3521 N>, <[DBT2008] UGC NNNN NN>, <[DBT2008] DDO NNNN NN>, N=933.
=E=	Catalogue in electronic form as J/AJ/135/823
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBT90]
[DBT90]	(De Geus+Bronfman+Thaddeus, 1990)
Write:	<<[DBT90] Complex N>> <<[DBT90] Cloud NN>>
N:	5+46
Object:	Cloud (SIMBAD class: MolCld = Molecular Cloud)
Note:	Fig.5: Map of CO complexes and clouds in Oph region.
in source:	NAME Ophiuchus Region
Ref:	=1990A&A...231..137D
by	DE GEUS E.J. , BRONFMAN L., THADDEUS P.
	Astron. Astrophys., 231, 137-150 (1990)
	A CO survey of the dark clouds in Ophiuchus.
o	Table 1: <[DBT90] Complex N> (Nos 1-5), <[DBT90] Cloud NN> (Nos 1-46).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBW97]
[DBW97]	(Duc+Brinks+Wink+, 1997)
Write:	<<[DBW97] HHMMSS.s+DDMMSS>>
N:	3
Object:	HI (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	Table 5: N=5 HI detections in the VLA field of APG 105.
in source:	APG 105
Ref:	=1997A&A...326..537D
by	DUC P.-A. , BRINKS E., WINK J.E., MIRABEL I.F.
	Astron. Astrophys., 326, 537-553 (1997)
	Gas segregation in the interacting system Arp 105.
o	APG 105S is defined as a Tidal dwarf Galaxy in 2000Natur.403..867B as [BLD2000] A105S.
o	Table 5: <[DBW97] HHMMSS.s+DDMMSS> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBY94]
[DBY94]	(Dobashi+Bernard+Yonekura+, 1994)
Write:	<<[DBY94] LLL.l+BB.b>> <<[DBY94] NNN>>
N:	159
Object:	Cloud (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Ref:	=1994ApJS...95..419D
by	DOBASHI K. , BERNARD J.-P., YONEKURA Y., FUKUI Y.
	Astrophys. J., Suppl. Ser., 95, 419-456 (1994)
	Molecular clouds in Cygnus. I. A large-scale survey.
o	<[DBY94] LLL.l+BB.b> N=159 = <[DBY94] NNN> (Nos 1-159).
=E=	Catalogue in electronic form as J/ApJS/95/419
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DBZ2015]
[DBZ2015]	(Diego+Broadhurst+Zitrin+, 2015) (Not yet in Simbad)
Write:	<<[DBZ2015] MACS J0717 NN.N>>
N:	102+33+24
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	N=102+33+24 gravitationally lensed images around the galaxy cluster MCS J0717.5+3745. Use of Hubble Frontier Fields (HFF) data. See also [ZBR2009], [LER2012], [RJL2014].
in source:	ClG J0717+3745 = MCS J0717.5+3745
Ref:	=2015MNRAS.451.3920D
by	DIEGO J.M. , BROADHURST T., ZITRIN A., LAM D., LIM J., FORD H.C., ZHENG W.
	Mon. Not. R. Astron. Soc., 451, 3920-3932 (2015)
	Hubble Frontier Field free-form mass mapping of the massive multiple-merging cluster MACSJ0717.5+3745.
o	Tables A1-A3: <[DBZ2015] MACS J0717 NN.N> (Nos 1.1-1.5 to 65.1-65.3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DC
DC	(Dottori+Carranza) (Not yet in Simbad)
*****	Avoid the usage of DC, prefer [DC71]
Origin	of the Acronym: L (1974Ap&SS..27....3M)
Details on Acronym: dc
dc	(dust cloud) (Not yet in Simbad)
*****	Avoid the usage of dc, prefer [H73]
Origin	of the Acronym: L (1998ApJ...499..209W)
Details on Acronym: DC
DC	(Delta Scuti)
*****	Avoid the usage of DC, prefer [BMF2002b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DC
DC	(Drake, Cluster)
*****	Avoid the usage of DC, prefer [D2005c]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DC
DC	(Dressler, Cluster)
*****	Avoid the usage of DC, prefer [D80]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: DC
DC	(Duerr+Craine)
*****	Avoid the usage of DC, prefer [DC82]
Origin	of the Acronym: L (2000A&A...353.1044H)
Details on Acronym: DC
DC	(Dark Cloud)
*****	Avoid the usage of DC, prefer DCld
Origin	of the Acronym: L = Found in the literature
Details on Acronym: DC
DC	(Dearborn obs., Catalog)
*****	Avoid the usage of DC, prefer DO
Details on Acronym: DC
DC	(Dressler, Cluster)
*****	Avoid the usage of DC, prefer DRCG
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DC
DC	(Dark Cloud)
*****	Avoid the usage of DC, prefer HMST
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DC
DC	(Double Compact)
Write:	<<NAME DC N>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=3 pairs of spherical compact galaxies. Finding charts
Ref:	=1976AN....297..275R
by	RICHTER N. , SCHNELL A.
	Astron. Nachr., 297, 275-278 (1976)
	Three new remarkable pairs of spherical compact galaxies.
o	<NAME DC N> (Nos DC 1 to DC 3)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DC2008]
[DC2008]	(Da Costa+Coleman, 2008)
Write:	<<[DC2008] NN-N-NNNNN>>
N:	4105+24
Object:	* in Cl* (SIMBAD class: Star)
Note:	AAT 2dF observations of the ome Cen Cluster.
in source:	ome Cen = NGC 5139
Ref:	=2008AJ....136..506D
by	DA COSTA G.S. , COLEMAN M.G.
	Astron. J., 136, 506-517 (2008)
	A spectroscopic survey for ω Centauri members at and beyond the cluster tidal radius.
o	tables 2-5: <[DC2008] NN-N-NNNNN> N=4105.
Ref:	=2012ApJ...751....6D
by	DA COSTA G.S.
	Astrophys. J., 751, 6 (2012)
	The dynamics of the outer parts of ω Centauri.
o	Tables 1-2: <[DC2008] NN-N-NNNNN> N=24 added, <[D2012] NNNNNN> N=34 among (Nos 44610-210569).
=E=	Catalogue in electronic form as <J/AJ/136/506/>
=E=	Catalogue in electronic form as J/ApJ/751/6
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DC71]
[DC71]	(Dottori+Carranza, 1971)= (DC) (Not yet in Simbad)
Write:	<<[DC71] LLL-N>>
N:	46
Object:	HII (SIMBAD class: HIIReg = HII Region)
Ref:	=1971Ap&SS..13..180D
by	DOTTORI H. , CARRANZA G.
	Astrophys. Space Sci., 13, 180-184 (1971)
	Interferometric study of the Milky Way between Carina and Aquila.
o	Table I: <[DC71] LLL-N> N=46
Origin	of the Acronym: L (1974Ap&SS..27....3M)
Details on Acronym: [DC78]
[DC78]	(Dressel+Condon, 1978)
Write:	<<[DC78] UGC NNNNNA>>
N:	2095
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Arecibo 2380MHz observations of bright galaxies selected from the Uppsala General Catalogue (UGC).
Ref:	=1978ApJS...36...53D
by	DRESSEL L.L. , CONDON J.J.
	Astrophys. J., Suppl. Ser., 36, 53-75 (1978)
	The Arecibo 2380 MHz survey of bright galaxies.
o	Table 2: <[DC78] UGC NNNNNA> N=2095.
=E=	Catalogue in electronic form as J/ApJS/36/53
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DC82]
[DC82]	(Duerr+Craine, 1982)= (DC)
Write:	<<[DC82] NNN>>
N:	144
Object:	Red * (SIMBAD class: Star)
Note:	N=144 red stars near LDN 1454. Finding charts in Figs 1.
Ref:	=1982PASP...94..567D
by	DUERR R. , CRAINE E.R.
	Publ. Astron. Soc. Pac., 94, 567-573 (1982)
	A catalog of red stars near L1454.
o	Table 1: <[DC82] NNN> (Nos 1-144).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: dC88
dC88	(da Costa+, 1988)
*****	Avoid the usage of dC88, prefer [DPS88]
Origin	of the Acronym: L (1997ApJ...491..421E)
Details on Acronym: [DC97]
[DC97]	(Dolgachev+Chernin, 1997)
Write:	<<[DC97] NN>>
N:	37
Object:	Cluster of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Supersedes Table 1 (1-18) and Table 2 (19-37) of 1995AZh....72..308T. No. 19 = No. 37 is certainly a misprint, certainly No. 1 of Table 2 in 1995AZh....72..308T. In 1995AZh....72..308T cross-id. with GHCG (Table 1) and MCL (Table 2)
Ref:	=1997ARep...41..284D
by	DOLGACHEV V.P. , CHERNIN A.D.
	Astron. Rep., 41, 284-290 (1997)
	Dynamics of wide galaxy triplets: numerical models and hidden mass estimates.
o	In the Table, No. 19 = No. 37, certainly a misprint, must be No. 1 of Table 2 in 1995AZh....72..308T, and [DC97] 19 = MCL 4
o	<[DC97] NN> (Nos 1-37)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCA2008]
[DCA2008]	(Di Carlo Corsi+Arkharov+, 2008) (Not yet in Simbad)
Write:	<<[DCA2008] N>>
N:	5
Object:	* (SIMBAD class: Star)
Note:	AZT-24 telescope observations of the field of SN 2006jc.
Ref:	=2008ApJ...684..471D
by	DI CARLO E. , CORSI C., ARKHAROV A.A., MASSI F., LARIONOV V.M., EFIMOVA N.V., DOLCI M., NAPOLEONE N., DI PAOLA A.
	Astrophys. J., 684, 471-480 (2008)
	Near-infrared observations of the type Ib supernova SN 2006jc: evidence of interactions with dust.
o	Parag. 2: Standard star AS 20 is [HMT98] AS 20-0 (= HD 80145)
o	Fig.1: <[DCA2008] N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCA2018]
[DCA2018]	(Duplancic+Coldwell+Alonso+, 2018)
Write:	<<[DCA2018] NNNNNN>>
N:	10929
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=10929 small galaxy systems, identified in SDSS DR14 data.
Ref:	=2018MNRAS.481.2458D
by	DUPLANCIC F. , COLDWELL G.V., ALONSO S., LAMBAS D.G.
	Mon. Not. R. Astron. Soc., 481, 2458-2469 (2018)
	On the nature of small galaxy systems.
o	<[DCA2018] NNNNNN> N=10929 among (Nos 14-422745).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: dCAZ94
dCAZ94	(de Carvalho+Zepf+, 1994)
Write:	<<dCAZ94 HCG NNN-NNa>>
N:	317
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Note:	ref. 1994ApJS...93...47D describes the catalogue of galaxies in Hickson HCG groups. ref. 1996ApJ...463L...5R gives a sample of galaxies in HCG 16 ref. 1997ApJS..110....1D present 317 galaxies in 17 HCGs. In the format 'HCG NNN-NNa' the letter 'a' stands for the letter of the galaxy in the HCG catalogue. ex.: dCAZ94 HCG 4-04 = dCAZ94 HCG 4-04c = HCG 4c
Ref:	=1996ApJ...463L...5R
by	RIBEIRO A.L.B. , DE CARVALHO R.R., COZIOL R., CAPELATO H.V., ZEPF S.E.
	Astrophys. J., 463, 5-8 (1996)
	HCG 16: a high concentration of active galaxies in the nearby universe.
o	Table 1: <dCAZ94 HCG 16-NN> N=7 among (Nos 1-10)
Ref:	=1997ApJS..110....1D
by	DE CARVALHO R.R. , RIBEIRO A.L.B., CAPELATO H.V., ZEPF S.E.
	Astrophys. J., Suppl. Ser., 110, 1-8 (1997)
	Redshift survey of galaxies around a selected sample of compact groups.
o	Table 2: <dCAZ94 HCG NN-NNa> N=317
=E=	Catalogue in electronic form as J/ApJS/110/1
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DCB2011]
[DCB2011]	(Devine+Chandler+Brogan+, 2011) (Not yet in Simbad)
Write:	<<[DCB2011] AN>>
N:	4+1+5
Object:	Dense Core (SIMBAD class: denseCore = Dense Core)
Note:	VLA NH3 and CCS line observations of MSXDC G019.27+0.07.
in source:	[PWC2006] NH3 G19.30+0.07
Ref:	=2011ApJ...733...44D
by	DEVINE K.E. , CHANDLER C.J., BROGAN C., CHURCHWELL E., INDEBETOUW R., SHIRLEY Y., BORG K.J.
	Astrophys. J., 733, 44 (2011)
	Very large array observations of the infrared dark cloud G19.30+0.07.
o	Figs 1+3: <[DCB2011] AN> (Nos C1-C4, S1, P1-P5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCB2017]
[DCB2017]	(Duronea+Cappa+Bronfman+, 2017)
Write:	<<[DCB2017] N>> <<[DCB2017] IRN>> <<[DCB2017] A>>
N:	4+3+2
Object:	Clump + (Rad) + (smm) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	ASTE CO(3-2) and HCO+(4-3) line observations of the HII region SH 2-39. Use of ATLASGAL, NVSS, MSX, Spitzer and WISE archival data.
in source:	SH 2-39
Ref:	=2017A&A...606A...8D
by	DURONEA N.U. , CAPPA C.E., BRONFMAN L., BORISSOVA J., GROMADZKI M., KUHN M.A.
	Astron. Astrophys., 606A, 8-8 (2017)
	Triggered massive star formation associated with the bubble HII region Sh2-39 (N5).
o	Tables 1-2: <[DCB2017] N> (Nos 1-4). Table 3: <[DCB2017] IRN> (Nos IR1-IR3). Table 4: <[DCB2017 A> (Nos A-B).
=E=	Catalogue in electronic form as <J/A+A/606/A8/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCC2003]
[DCC2003]	(Ding+Charlton+Churchill+, 2003)
Write:	<<[DCC2003] GN>>
N:	4
Object:	G (SIMBAD class: Galaxy)
Note:	WIYN observations. N=4 galaxies in the field of PG 1206+459.
Ref:	=2003ApJ...590..746D
by	DING J. , CHARLTON J.C., CHURCHILL C.W., PALMA C.
	Astrophys. J., 590, 746-769 (2003)
	The multiphase absorption systems toward PG 1206+459.
o	Systems A, B, C are identified in SIMBAD as [RKV2003] QSO J1208+4540 abs 0.9254, [RKV2003] QSO J1208+4540 abs 0.9277, [RCC2002] QSO J1208+4540 abs 0.9343.
o	Fig.4, Table 2: <[DCC2003] GN> (Nos G1-G4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCD2013]
[DCD2013]	(Drake+Catelan+Djorgovski+, 2013)= (CSS)
Write:	<<[DCD2013] CSS JHHMMSS.s+DDMMSS>> <<[DCD2013] MLS JHHMMSS.s+DDMMSS>>
N:	12227+2040+1207
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Note:	N=12227+2040+1207 RR Lyrae from the Catalina Surveys Data Release 1 (see http://nesssi.cacr.caltech.edu/DataRelease/index1.html and also http://nesssi.cacr.caltech.edu/DataRelease/RRL.html), that used observations from the Catalina Sky Survey 0.7m Schmidt (CSS), and Mt. Lemmon Survey 1.5m Cass (MLS) telescopes.
Ref:	=2013ApJ...763...32D
by	DRAKE A.J. , CATELAN M., DJORGOVSKI S.G., TORREALBA G., GRAHAM M.J., BELOKUROV V., KOPOSOV S.E., MAHABAL A., PRIETO J.L., DONALEK C., WILLIAMS R., LARSON S., CHRISTENSEN E., BESHORE E.
	Astrophys. J., 763, 32 (2013)
	Probing the outer galactic halo with RR Lyrae from the Catalina surveys.
o	Tables 1-2: <[DCD2013] CSS JHHMMSS.s+DDMMSS> N=12227.
Ref:	=2013ApJ...765..154D
by	DRAKE A.J. , CATELAN M., DJORGOVSKI S.G., TORREALBA G., GRAHAM M.J., MAHABAL A., PRIETO J.L., DONALEK C., WILLIAMS R., LARSON S., CHRISTENSEN E., BESHORE E.
	Astrophys. J., 765, 154 (2013)
	Evidence for a Milky way tidal stream reaching beyond 100 kpc.
o	Table 1: <[DCD2013] MLS JHHMMSS.s+DDMMSS> N=1207. Table 2: <[DCD2013] CSS JHHMMSS.s+DDMMSS> N=2040.
=E=	Catalogue in electronic form as <J/ApJ/765/154/>
=E=	Catalogue in electronic form as <J/ApJ/763/32/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCD2015]
[DCD2015]	(De Silva+Carraro+D'orazi+, 2015)
Write:	<<[DCD2015] NNNN>>
N:	22
Object:	* (SIMBAD class: Star)
Note:	AAT 3.9m telescope HERMES photometric observations and Las Campanas 1.0m Swope telescope CDD photometry observations of N=22 stars in the open cluster Trumpler 22.
in source:	Cl Trumpler 22
Ref:	=2015MNRAS.453..106D
by	DE SILVA G.M. , CARRARO G., D'ORAZI V., EFREMOVA V., MacPHERSON H., MARTELL S., RIZZO L.
	Mon. Not. R. Astron. Soc., 453, 106-112 (2015)
	Binary open clusters in the Milky Way: photometric and spectroscopic analysis of NGC 5617 and Trumpler 22.
o	Table 2: <[DCD2015] NNNN> N=22 among (Nos 794-1417).
=E=	Catalogue in electronic form as <J/MNRAS/453/106/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCE2008]
[DCE2008]	(Dunham+Crapsi+Evans+, 2008)
Write:	<<[DCE2008] NNN>>
N:	218
Object:	Protostar (SIMBAD class: YSO = Young Stellar Object)
Note:	Spitzer Space Telescope c2d observations.
Ref:	=2008ApJS..179..249D
by	DUNHAM M.M. , CRAPSI A., EVANS II N.J., BOURKE T.L., HUARD T.L., MYERS P.C., KAUFFMANN J.
	Astrophys. J., Suppl. Ser., 179, 249-282 (2008)
	Identifying the low-luminosity population of embedded protostars in the c2d observations of clouds and cores.
o	Tables 2-8: <[DCE2008] NNN> (Nos 1-218).
=E=	Catalogue in electronic form as J/ApJS/179/249
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCF2017]
[DCF2017]	(Ding+Cai+Fan+, 2017)
Write:	<<[DCF2017] N>> <<[DCF2017] Ding-N>> (not recognised by Simbad, but found in literature)
N:	5
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC3 observations of N=5 galaxies at z=5.7 in the SDF and SXDF fields.
in source:	NAME SXDF
in source:	NAME SDF
Ref:	=2017ApJ...838L..22D
by	DING J. , CAI Z., FAN X., STARK D.P., BIAN F., JIANG L., McGREER I.D., ROBERTSON B.E., SIANA B.
	Astrophys. J., 838L, 22-22 (2017)
	Constraining C III] emission in a sample of five luminous z = 5.7 galaxies.
o	Tables 1-2: <[DCF2017] N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCG2005]
[DCG2005]	(de Ugarte Postigo+Castro-Tirado+Gorosabel+, 2005)= ([DCG2005a]) (Not yet in Simbad)
Write:	<<[DCG2005] NN>>
N:	10
Object:	* (SIMBAD class: Star)
Note:	N=10 calibration stds in the field of GRB 021004.
Ref:	=2005A&A...443..841D
by	DE UGARTE POSTIGO A. , CASTRO-TIRADO A.J., GOROSABEL J., JOHANNESSON G., BJOERNSSON G., GUDMUNDSSON E.H., BREMER M., PAK S., TANVIR N., CASTRO CERON J.M., GUZYI S., JELINEK M., KLOSE S., PEREZ-RAMIREZ D., ACEITUNO J., CAMPO BAGATIN A., COVINO S., CARDIEL N., FATHKULLIN T., HENDEN A.A., HUFERATH S., KURATA Y., MALESANI D., MANNUCCI F., RUIZ-LAPUENTE P., SOKOLOV V., THIELE U., WISOTZKI L., ANTONELLI L.A., BARTOLINI C., BOATTINI A., GUARNIERI A., PICCIONI A., PIZZICHINI G., DEL PRINCIPE M., DI PAOLA A., FUGAZZA D., GHISELLINI G., HUNT L., KONSTANTINOVA T., MASETTI N., PALAZZI E., PIAN E., STEFANON M., TESTA V., TRISTRAM P.J.
	Astron. Astrophys., 443, 841-849 (2005)
	GRB 021004 modelled by multiple energy injections.
o	Fig.1, Table 1: <[DCG2005] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCG2005a]
[DCG2005a]	(de Ugarte Postigo+Castro-Tirado+Gorosabel+, 2005) (Not yet in Simbad)
*****	Avoid the usage of [DCG2005a], prefer [DCG2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCG2005b]
[DCG2005b]	(De Gregorio-Montsalvo+Chandler+Gomez+, 2005) (Not yet in Simbad)
Write:	<<[DCG2005b] JHHMMSS.ss+DDMMSS.s>> <<[DCG2005b] JHHMMSS.sss+DDMMSS.ss>>
N:	23+11+24
Object:	H2O Maser (SIMBAD class: Maser)
Note:	H2O maser components in the environment of [HKM99] B1-IRS.
Ref:	=2005ApJ...628..789D
by	DE GREGORIO-MONSALVO I. , CHANDLER C.J., GOMEZ J.F., KUIPER T.B.H., TORRELLES J.M., ANGLADA G.
	Astrophys. J., 628, 789-799 (2005)
	High-resolution molecular line observations of the environment of the class 0 source B1-IRS.
o	Tables 1, 2, 3: <[DCG2005b] JHHMMSS.ss+DDMMSS.s>, <[DCG2005b] JHHMMSS.sss+DDMMSS.ss>, N=23+11+24.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCG2005c]
[DCG2005c]	(de Ugarte Postigo+Castro-Tirado+Guzily+, 2005)
Write:	<<[DCG2005c] N>>
N:	3
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Optical observations at the 1.5m OSN telescope at the Observatorio de Sierra Nevada. N=3 sources in the field of GRB 051006.
Ref:	=2005GCN..4064....1D
by	DE UGARTE POSTIGO A. , CASTRO-TIRADO A.J., GUZIY S., CASANOVA V., JELINEK M., GOROSABEL J.
	GRB Coordinates Network, Circular Service, 4064, 1-None (2005)
	GRB 051006: optical observations at sierra nevada.
o	<[DCG2005c] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCG2014]
[DCG2014]	(Dowell+Conley+Glenn+, 2014)
Write:	<<[DCG2014] GOODSN N>> <<[DCG2014] FLS NN>> <<[DCG2014] LSW NNN>>
N:	1+18+21
Object:	IRAS G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Herschel SPIRE 250-500µm observations of N=38 high-z galaxies.
Ref:	=2014ApJ...780...75D
by	DOWELL C.D. , CONLEY A., GLENN J., ARUMUGAM V., ASBOTH V., AUSSEL H., BERTOLDI F., BETHERMIN M., BOCK J., BOSELLI A., BRIDGE C., BUAT V., BURGARELLA D., CABRERA-LAVERS A., CASEY C.M., CHAPMAN S.C., CLEMENTS D.L., CONVERSI L., COORAY A., DANNERBAUER H., DE BERNARDIS F., ELLSWORTH-BOWERS T.P., FARRAH D., FRANCESCHINI A., GRIFFIN M., GURWELL M.A., HALPERN M., HATZIMINAOGLOU E., HEINIS S., IBAR E., IVISON R.J., LAPORTE N., MARCHETTI L., MARTINEZ-NAVAJAS P., MARSDEN G., MORRISON G.E., NGUYEN H.T., O'HALLORAN B., OLIVER S.J., OMONT A., PAGE M.J., PAPAGEORGIOU A., PEARSON C.P., PETITPAS G., PEREZ-FOURNON I., POHLEN M., RIECHERS D., RIGOPOULOU D., ROSEBOOM I.G., ROWAN-ROBINSON M., SAYERS J., SCHULZ B., SCOTT D., SEYMOUR N., SHUPE D.L., SMITH A.J., STREBLYANSKA A., SYMEONIDIS M., VACCARI M., VALTCHANOV I., VIEIRA J.D., VIERO M., WANG L., WARDLOW J., XU C.K., ZEMCOV M.
	Astrophys. J., 780, 75 (2014)
	HerMES: candidate high-redshift galaxies discovered with Herschel/SPIRE.
o	Table 2: <[DCG2014] GOODSN N> (No 8), Table 2: <[DCG2014] FLS NN> N=18 (Nos 1-34), Table 2: <[DCG2014] LSW NNN> N=21 (Nos 20-102).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCH2013]
[DCH2013]	(Doerr+Chini+Haas+, 2013)
Write:	<<[DCH2013] NNNN>>
N:	139
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	N=139 variable stars in RCW 38 using NIR observations with the 80cm IRIS telescope near Cerro Armazones, Chile.
in source:	RCW 38
Ref:	=2013A&A...553A..48D
by	DOERR M. , CHINI R., HAAS M., LEMKE R., NUERNBERGER D.
	Astron. Astrophys., 553A, 48-48 (2013)
	Near-infrared variability in the star-forming region RCW 38.
o	Tables 1-2: <[DCH2013] NNNN> N=139 among (Nos 23-1652).
=E=	Catalogue in electronic form as J/A+A/553/A48
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCI2008]
[DCI2008]	(Devine+Churchwell+Indebetouw+, 2008)
N:	186
Object:	Poss. YSO + * (SIMBAD class: Star)
Note:	WIYN 3.5-m telescope Near-Infrared Imager (NIRIM) camera JHK photometric observations of N=186 stars in N=3 massive star-forming regions.
in source:	RAFGL 437
in source:	RAFGL 5142
in source:	RAFGL 5180
Ref:	=2008AJ....135.2095D
by	DEVINE K.E. , CHURCHWELL E.B., INDEBETOUW R., WATSON C., CRAWFORD S.M.
	Astron. J., 135, 2095-2107 (2008)
	A WIYN near-infrared investigation of three massive star-forming regions.
o	Table 2: <[DCI2008] AFGL437 NN> (Nos 1-48), <[DCI2008] AFGL5180 NN> (Nos 1-83), <[DCI2008] AFGL5142 NN> (Nos 1-55).
=E=	Catalogue in electronic form as J/AJ/135/2095
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: DCL
DCL	(Dickens+Currie+Lucey)
*****	Avoid the usage of DCL, prefer [DCL86]
Origin	of the Acronym: L (1997A&AS..124....1J)
Details on Acronym: [DCL2021]
[DCL2021]	(Durret+Chiche+Lobo+, 2021)
Write:	<<[DCL2021] MACS J0717.5+3745 NN>> <<[DCL2021] Cl 0016+16 a>> <<[DCL2021] Cl0152.7-1357 a>> <<[DCL2021] Abell NNN a>> <<[DCL2021] MACS JHHMM.m+DDMM a>> <<[DCL2021] LCDCS NNNN a>> <<[DCL2021] MJM98 34 a>> <<[DCL2021] 3C 295 a>> <<[DCL2021] RX JHHMM.m+DDMM a>> <<[DCL2021] MS HHMM.m+DDMM a>>
N:	81+8+6+15+24+24+1+8+7+4
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=81+97 jellyfish galaxy candidates in the extended region around MCS J0717.5+3745 and in 22 other clusters. Use of HST archival data.
Ref:	=2021A&A...648A..63D
by	DURRET F. , CHICHE S., LOBO C., JAUZAC M.
	Astron. Astrophys., 648A, 63-63 (2021)
	Jellyfish galaxy candidates in MACS J0717.5+3745 and 39 other clusters of the DAFT/FADA and CLASH surveys.
o	galaxy C153 is [OKL2005] 47 in SIMBAD
o	Figs A.1-A.9, Table 2: <[DCL2021] MACS J0717.5+3745 NN> (Nos 1-81). Figs B.1-B.22, Table 3: <[DCL2021] Cl 0016+16 a> (Nos a-h), <[DCL2021] Cl0152.7-1357 a> (Nos a-f), <[DCL2021] Abell NNN a> N=2+2+11, <[DCL2021] MACS JHHMM.m+DDMM a> N=8+2+5+4+3+2, <[DCL2021] LCDCS NNNN a> N=9+7+1+7, <[DCL2021] MJM98 34 a> (No. a), <[DCL2021] 3C 295 a> (Nos a-h), <[DCL2021] RX JHHMM.m+DDMM a> N=1+1+5, <[DCL2021] MS HHMM.m+DDMM a> N=3+1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCL86]
[DCL86]	(Dickens+Currie+Lucey, 1986)= (DCL)
Write:	<<[DCL86] NNN>>
N:	570
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Table 11: (Nos 1-572), Nos 110 and 203 missing
in source:	Centaurus Cluster = ACO 3526
Ref:	=1986MNRAS.220..679D
by	DICKENS R.J. , CURRIE M.J., LUCEY J.R.
	Mon. Not. R. Astron. Soc., 220, 679-711 (1986)
	The Centaurus cluster of galaxies. I. The data.
o	Table 11: <[DCL86] NNN> N=570 among 572
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCL88]
[DCL88]	(Deharveng+Caplan+Lequeux+, 1988)
Write:	<<[DCL88] NNNA>>
N:	176
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Format NNNA, (Nos 1-159)
in source:	NGC 300
Ref:	=1988A&AS...73..407D
by	DEHARVENG L. , CAPLAN J., LEQUEUX J., AZZOPARDI M., BREYSACHER J., TARENGHI M., WESTERLUND B.
	Astron. Astrophys., Suppl. Ser., 73, 407-423 (1988)
	H II regions in NGC 300.
o	<[DCL88] NNNA> N=176, (Nos 1-159)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCL91]
[DCL91]	(De Lara+Chavarria-K.+Lopez-Molina, 1991)= (IRS)
Write:	<<[DCL91] IRS NN>>
N:	10
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	See also [CDF88]
in source:	NAME Serpens Cloud
Ref:	=1991A&A...243..139D
by	DE LARA E. , CHAVARRIA-K C., LOPEZ-MOLINA G.
	Astron. Astrophys., 243, 139-142 (1991)
	Distance to the Serpens cloud. II.
o	Table 2: <[CDF88] HA NNW> (Nos 4N, 4S, 7N, 7S). Table 4: <[DCL91] IRS NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCL92]
[DCL92]	(Deharveng+Caplan+Lombard, 1992)
Write:	<<[DCL92] NNN>>
N:	362
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	* in the LMC Henize HII region N 159A.
in source:	Magellanic Clouds:LMC:LHA 120-N 159A = LHA 120-N 159A
Ref:	=1992A&AS...94..359D
by	DEHARVENG L. , CAPLAN J., LOMBARD J.
	Astron. Astrophys., Suppl. Ser., 94, 359-375 (1992)
	Photometry of the LMC HII region N 156A and of its stellar content. Stellar observations and reductions.
o	(Erratum) erratum vol. 95, p 389 + 601
o	misprint in the title: N156A for N159A (LHA 120-N 159A)
o	<[DCL92] NNN> (Nos 1-362).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DCld
DCld	(Dark Cloud)= (DC)
Write:	<<DCld LLL.l+BB.b>>
Object:	Dark Cloud + Globule (SIMBAD class: Cloud)
Note:	Systematic designation, in SIMBAD only.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCM2005]
[DCM2005]	(Di Fabrizio+Clementini+Maio+, 2005)= ([GBC2004b])
Write:	<<[DCM2005] A-NNNNN>> <<[DCM2005] B-NNNNN>> <<[DCM2005] AN-NNNNN>> (not recognised by Simbad, but found in literature) <<[DCM2005] BN-NNNNN>>
N:	101+171
Object:	V* (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT spectroscopy of RR Lyrae and photometric observations with the 1.54m Danish telescope at La Silla. Search for V* in two areas A and B close to the LMC Bar. In the first ref. 2004A&A...421..937G, the authors divided the areas A and B into sub-areas A1 to A4, and B1 to B4, but these sub-divisions are not used in the second ref. 2005A&A...430..603D.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2004A&A...421..937G
by	GRATTON R.G. , BRAGAGLIA A., CLEMENTINI G., CARRETTA E., DI FABRIZIO L., MAIO M., TARIBELLO E.
	Astron. Astrophys., 421, 937-952 (2004)
	Metal abundances of RR Lyrae stars in the bar of the Large Magellanic Cloud.
o	Table 3: star 99999 not identified. Table 7: Authors say 'variables identified acording to Di Fabrizio+', ref. 2005A&A...430..603D ([DCM2005]), so the format is 'A-NNNNN' (for fields A and B), sub-fields 'AN' are not used.
o	<Table 7: <[DCM2005] A-NNNNN> N=101.
Ref:	=2005A&A...430..603D
by	DI FABRIZIO L. , CLEMENTINI G., MAIO M., BRAGAGLIA A., CARRETTA E., GRATTON R., MONTEGRIFFO P., ZOCCALI M.
	Astron. Astrophys., 430, 603-628 (2005)
	Variable stars in the bar of the Large Magellanic Cloud: The photometric catalogue.
o	Table 5: <[DCM2005] A-NNNNN> N=104. Table 6: <[DCM2005] B-NNNNN> N=77.
=E=	Catalogue in electronic form as J/A+A/430/603
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCM2007]
[DCM2007]	(Djorgovski+Courbin+Meylan+, 2007)= ([DCM2007a])
Write:	<<[DCM2007] QSO JHHMM+DDMMA abs N.NNN>> <<[DCM2007] QSO JHHMM+DDMMA abs N.NNNN>> <<[DCM2007] QQQ J1432-0106>> <<[DCM2007] QQQ J1432-0106>> (not recognised by Simbad, but found in literature)
N:	2+2+1+1
Object:	Triple quasar + Absorber (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Keck LRIS observations of the field of LBQS 1429-0053.
Ref:	=2007ApJ...662L...1D
by	DJORGOVSKI S.G. , COURBIN F., MEYLAN G., SLUSE D., THOMPSON D., MAHABAL A., GLIKMAN E.
	Astrophys. J., 662L, 1-5 (2007)
	Discovery of a probable physical triple quasar.
o	In text, APM 08729+5255 is a misprint for APM 08279+5255
o	Text: <[DCM2007] QQQ J1432-0106> N=1, <[DCM2007] QSO JHHMM+DDMMA abs N.NNN>, <[DCM2007] QSO JHHMM+DDMMA abs N.NNNN>, N=2+2+1. Fig.1: <[FAG2003] N> (Nos 8, 9) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCM2007a]
[DCM2007a]	(Djorgovski+Courbin+Meylan+, 2007) (Not yet in Simbad)
*****	Avoid the usage of [DCM2007a], prefer [DCM2007]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCM2007b]
[DCM2007b]	(Dunlop+Cirasuolo+McCLure, 2007)
Write:	<<[DCM2007b] NNNN>>
N:	19
Object:	G (SIMBAD class: Galaxy)
Note:	Search for massive galaxies in the GOODS South Field. Use of archival HST ACS and VLT ISAAC data.
Ref:	=2007MNRAS.376.1054D
by	DUNLOP J.S. , CIRASUOLO M., McLURE R.J.
	Mon. Not. R. Astron. Soc., 376, 1054-1064 (2007)
	A systematic search for very massive galaxies at z > 4.
o	Tables 3,4,5: <[DCM2007b] NNNN> N=19 among (Nos 1865-3122).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCM2011]
[DCM2011]	(D'avanzo+Campana+Munoz-Darias+, 2011)
Write:	<<[DCM2011] NN>>
N:	41
Object:	(NIR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Stat:	is completely incorporated in Simbad
Note:	VLT NACO NIR observations of N=41 possible counterparts of SWIFT J1749.4-2807.
Ref:	=2011A&A...534A..92D
by	D'AVANZO P. , CAMPANA S., MUNOZ-DARIAS T., BELLONI T., BOZZO E., FALANGA M., STELLA L.
	Astron. Astrophys., 534A, 92-92 (2011)
	A search for the near-infrared counterpart of the eclipsing millisecond X-ray pulsar Swift J1749.4-2807.
o	Table 2: <[DCM2011] NN> (Nos 1-41).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCM91]
[DCM91]	(Dewdney+Costain+McHardy+, 1991)
Write:	<<[DCM91] HHMM+DD RNN>> <<[DCM91] HHMM+DD XN>>
N:	38+3
Object:	(Rad) + (X) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Radio-sources and X-ray sources in 2 fields. map of each field See also Paper I: [HMW88]
Ref:	=1991ApJS...76.1055D
by	DEWDNEY P.E. , COSTAIN C.H., McHARDY I., WILLIS A.G., HARRIS D.E., STERN C.P.
	Astrophys. J., Suppl. Ser., 76, 1055-1066 (1991)
	An X-ray and radio study of steep-spectrum radio sources. II. Four fields from a 22 MHz polar cap survey.
o	Table 2: <[DCM91] 0506+77 RNN> (Nos R1-R18). Table 3: <[DCM91] 0506+77 XN> (Nos X1-X3). Table 4: <[DCM91] 0917+75 RNN> (Nos R1-R20).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DCMC
DCMC	(DENIS Catalogue of the Magellanic Clouds)
Write:	<<DCMC JHHMMSS.ss+DDMMSS.s>>
N:	1314009+318631
Object:	* (SIMBAD class: Star)
Note:	first version of a complete near infrared Point Source Catalogue (PSC) towards the Magellanic Clouds (MCs) extracted from the data obtained with the Deep Near Infrared Survey of the Southern Sky - DENIS (Epchtein+ 1997Msngr..87...27E) The catalogue covers an area of 19.87times 16sq.deg centered on 5 27 20 -69 00 00 for the LMC, and 14.7times 10sq.deg centered on 1 02 40 -73 00 00 for the SMC. It contains 1314009 sources towards the LMC and 318631 sources towards the SMC each detected in at least 2 of the 3 photometric bands involved in the survey. 70per100 of the detected sources are real members of the MCs respectively, and consist mainly of red giants, asymptotic giant branch stars and supergiants. The observations have all been made with the same instrument and therefore provide a homogeneous set of photometric data. Available at: http://cdsweb.u-strasbg.fr/denis.html
Ref:	=2000A&AS..144..235C
by	CIONI M.-R. , LOUP C., HABING H.J., FOUQUE P., BERTIN E., DEUL E., EGRET D., ALARD C., DE BATZ B., BORSENBERGER J., DENNEFELD M., EPCHTEIN N., FORVEILLE T., GARZON F., HRON J., KIMESWENGER S., LACOMBE F., LE BERTRE T., MAMON G.A., OMONT A., PATUREL G., PERSI P., ROBIN A., ROUAN D., SIMON G., TIPHENE D., VAUGLIN I., WAGNER S.
	Astron. Astrophys., Suppl. Ser., 144, 235-245 (2000)
	The DENIS Point Source Catalogue towards the Magellanic Clouds.
o	Table 7: <DCMC JHHMMSS.ss+DDMMSS.s> N=1314009+318631.
=E=	Catalogue in electronic form as II/228
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [DCN2010]
[DCN2010]	(Dougherty+Clark+Negueruela+, 2010)= (D09)
Write:	<<[DCN2010] D09-RN>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ATCA 3, 6, 13, and 20cm continuum observations of Cl Westerlund 1.
in source:	Cl Westerlund 1
Ref:	=2010A&A...511A..58D
by	DOUGHERTY S.M. , CLARK J.S., NEGUERUELA I., JOHNSON T., CHAPMAN J.M.
	Astron. Astrophys., 511A, 58-58 (2010)
	Radio emission from the massive stars in the galactic super star cluster Westerlund 1.
o	Fig. 2, Table 2: <[DCN2010] D09-RN> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCO2008]
[DCO2008]	(Devor+Charbonneau+O'Donovan+, 2008)
Write:	<<[DCO2008] T-CCCN-NNNNN>>
N:	773
Object:	EB* (SIMBAD class: EclBin = Eclipsing Binary)
Stat:	is completely incorporated in Simbad
Note:	TrES survey is used to identified eclipsing binary systems.
Ref:	=2008AJ....135..850D
by	DEVOR J. , CHARBONNEAU D., O'DONOVAN F.T., MANDUSHEV G., TORRES G.
	Astron. J., 135, 850-877 (2008)
	Identification, classifications, and absolute properties of 773 eclipsing binaries found in the trans-atlantic exoplanet survey.
o	Tables 3-10: <[DCO2008] T-CCCN-NNNNN> N=773.
=E=	Catalogue in electronic form as J/AJ/135/850
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCP2004]
[DCP2004]	(Dessauges-Zavadsky+Calura+Prochaska+, 2004)
Write:	<<[DCP2004] QSO JHHMM+DDMM abs N.NNNNNN>>
N:	7+17+30+38
Object:	Absorber
Note:	UVES-VLT spectra combined with existing HIRES-Keck spectra. See also Paper II: [DPD2006].
Ref:	=2004A&A...416...79D
by	DESSAUGES-ZAVADSKY M. , CALURA F., PROCHASKA J.X., D'ODORICO S., MATTEUCCI F.
	Astron. Astrophys., 416, 79-110 (2004)
	A comprehensive set of elemental abundances in damped Lyα systems: Revealing the nature of these high-redshift galaxies.
o	QSO 2343+12 = QSO J2346+1248 = QSO J2346+1241. Table 1: The DLAs in the line of sight of the 4 QSOs are [PGW2001] QSO JHHMM+DDMM abs N.NNN in SIMBAD.
o	Table 3: <[DCP2004] QSO J0103+1316 abs N.NNNNNN> N=7. Table 4: <[DCP2004] QSO J1333+1649 abs N.NNNNNN> N=17. Table 5: <[DCP2004] QSO J2234+0000 abs N.NNNNNN> N=30. Tables6, 7: <[DCP2004] QSO J2346+1248 abs N.NNNNNN> N=23+15.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCP91]
[DCP91]	(Davoust+Considere+Poulain, 1991)
Write:	<<[DCP91] GN>>
N:	5
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=5 galaxies in the group of G 'Anon 0021+25' (Nos G1-G5), G1 is a Seyfert galaxy, G2-G4 are companions Map fig.1
in source:	Anon 0021+25
Ref:	=1991A&A...252...69D
by	DAVOUST E. , CONSIDERE S., POULAIN P.
	Astron. Astrophys., 252, 69-74 (1991)
	Discovery of a ring Seyfert in a group of galaxies.
o	<[DCP91] GN> (Nos G1-G5). <Anon 0021+25>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCP93]
[DCP93]	(De Juan+Colina+Perez-Fournon, 1993)
Write:	<<[DCP93] 3C NNNA>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Companion galaxy of the 2 radio-galaxies 3C 449 and 3C 465 are designated as 3C 449B and 3C 465B by the authors.
Ref:	=1993Ap&SS.205..209D
by	DE JUAN L. , COLINA L., PEREZ-FOURNON I.
	Astrophys. Space Sci., 205, 209-216 (1993)
	Structure of interacting elliptical radio galaxies.
o	Table II: <[DCP93] 3C 449B> N=1, <[DCP93] 3C 465B> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCP96]
[DCP96]	(Di Nella+Couch+Paturel+, 1996)
Write:	<<[DCP96] HHMMSS.ss+DDMMSS.s>>
N:	379
Object:	G (SIMBAD class: Galaxy)
Ref:	=1996MNRAS.283..367D
by	DI NELLA H. , COUCH W.J., PATUREL G., PARKER Q.A.
	Mon. Not. R. Astron. Soc., 283, 367-380 (1996)
	Are the Perseus-Pisces chain and the Pavo-Indus wall connected?
o	Table 3: internal format in col.(3) not used in SIMBAD
o	Table 3: <[DCP96] HHMMSS.ss-DDMMSS.s> N=379
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCP97]
[DCP97]	(Di Nella+Couch+Parker+, 1997)
Write:	<<[DCP97] HHMMSS.ss+DDMMSS.s>>
N:	210
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Ref:	=1997MNRAS.287..472D
by	DI NELLA H. , COUCH W.J., PARKER Q.A., PATUREL G.
	Mon. Not. R. Astron. Soc., 287, 472-480 (1997)
	Unveiling a connection between large-scale structures behind the southern Milky Way.
o	Table 3: <[DCP97] HHMMSS.ss+DDMMSS.s> N=210
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCR2004]
[DCR2004]	(Daddi+Cimatti+Renzini+, 2004)= ([DCR2004a]) = (K20)
Write:	<<[DCR2004] N>>
N:	9
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	GOODS (Great Observatories Origins Deep Survey) South Field search for starburst galaxies at z > 1.7. New VLT FORS2 observations in the K20 survey region are combined with HST ACS and VLT ISAAC observations.
in source:	NAME GOODS South Field
Ref:	=2004ApJ...600L.127D
by	DADDI E. , CIMATTI A., RENZINI A., VERNET J., CONSELICE C., POZZETTI L., MIGNOLI M., TOZZI P., BROADHURST T., DI SEREGO ALIGHIERI S., FONTANA A., NONINO M., ROSATI P., ZAMORANI G.
	Astrophys. J., 600, 127-130 (2004)
	Near-infrared bright galaxies at z≃2. Entering the spheroid formation epoch?.
o	Table 1: <[DCR2004] N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCR2004a]
[DCR2004a]	(Daddi+Cimatti+Renzini+, 2004)
*****	Avoid the usage of [DCR2004a], prefer [DCR2004]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCR2004b]
[DCR2004b]	(D'Odorico+Cristiani+Romano+, 2004)
Write:	<<[DCR2004b] QSO JHHMM+DDMM abs N.NNN>> <<[DCR2004b] QSO JHHMM+DDMM abs N.NNNN>>
N:	2+6
Object:	Absorber
Note:	VLT UVES observations: Absorption systems in 6 QSOs.
Ref:	=2004MNRAS.351..976D
by	D'ODORICO V. , CRISTIANI S., ROMANO D., GRANATO G.L., DANESE L.
	Mon. Not. R. Astron. Soc., 351, 976-988 (2004)
	Chemical abundances in QSO host galaxies and environments from narrow absorption line systems.
o	(Erratum) erratum vol. 355, p. 1399 (2004)
o	Table 9: <[DCR2004b] QSO JHHMM+DDMM abs N.NNN>, <[DCR2004b] QSO JHHMM+DDMM abs N.NNNN>, N=2+6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCR2008]
[DCR2008]	(DOng+Calzetti+Regan+, 2008)
Write:	<<[DCR2008] NNN>>
N:	152
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Spitzer IRAC observations of M 83.
in source:	M 83 = NGC 5236
Ref:	=2008AJ....136..479D
by	DONG H. , CALZETTI D., REGAN M., THILKER D., BIANCHI L., MEURER G.R., WALTER F.
	Astron. J., 136, 479-497 (2008)
	Spitzer observations of star formation in the extreme outer disk of M83 (NGC5236).
o	Table 2: <[DCR2008] NNN> (Nos 1-152).
=E=	Catalogue in electronic form as <J/AJ/136/479/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCS2002]
[DCS2002]	(Dietrich+Clowe+Soucail, 2002)
Write:	<<[DCS2002] NNN>>
N:	202
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Spectroscopic catalog of the neighboring massive clusters ACO 222 and ACO 223.
in source:	ACO 222
in source:	ACO 223
Ref:	=2002A&A...394..395D
by	DIETRICH J.P. , CLOWE D.I., SOUCAIL G.
	Astron. Astrophys., 394, 395-403 (2002)
	Spectroscopy of the neighboring massive clusters Abell 222 and Abell 223.
o	Catalog: <[DCS2002] NNN> (Nos 1-202).
=E=	Catalogue in electronic form as J/A+A/394/395
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCS2011]
[DCS2011]	(Duc+Cuillandre+Serra+, 2011)
Write:	<<[DCS2011] TDG N-W>>
N:	3
Object:	Tidal dwarf galaxy candidate (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	CFHT MegaCam (g'r'i') observations of N=3 tidal dwarf galaxies (TDG) in NGC 5557. Use of WSRT HI and GALEX data.
in source:	NGC 5557
Ref:	=2011MNRAS.417..863D
by	DUC P.-A. , CUILLANDRE J.-C., SERRA P., MICHEL-DANSAC L., FERRIERE E., ALATALO K., BLITZ L., BOIS M., BOURNAUD F., BUREAU M., CAPPELLARI M., DAVIES R.L., DAVIS T.A., DE ZEEUW P.T., EMSELLEM E., KHOCHFAR S., KRAJNOVIC D., KUNTSCHNER H., LABLANCHE P.-Y., McDERMID R.M., MORGANTI R., NAAB T., OOSTERLOO T., SARZI M., SCOTT N., WEIJMANS A.-M., YOUNG L.M.
	Mon. Not. R. Astron. Soc., 417, 863-881 (2011)
	The ATLAS^{3D} project – IX. The merger origin of a fast- and a slow-rotating early-type galaxy revealed with deep optical imaging: first results.
o	Figs 5+7, Table 2: <[DCS2011] TDG N-W> (Nos 1-E, 2-E, 3-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCS2017]
[DCS2017]	(Djupvik+Comeron+Schneider, 2017)
Write:	<<[DCS2017] NNN>>
N:	144
Object:	Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Stat:	is completely incorporated in Simbad
Note:	Calar Alto 3.5m telescope OMEGA2000 NIR and IAC80 CAMELOT photometric observations of N=144 young stellar objects in the globule IRAS 20319+3958. Use of archival Spitzer IRAC data.
in source:	IRAS 20319+3958
Ref:	=2017A&A...599A..37D
by	DJUPVIK A.A. , COMERON F., SCHNEIDER N.
	Astron. Astrophys., 599A, 37-37 (2017)
	Globules and pillars in Cygnus X. II. Massive star formation in the globule IRAS 20319+3958.
o	Table 3: <[DCS2017] NNN> (Nos 1-144).
=E=	Catalogue in electronic form as J/A+A/599/A37
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCT2000]
[DCT2000]	(Diaz+Castellanos+Terlevich+, 2000) (Not yet in Simbad)
Write:	<<[DCT2000] AAN>>
N:	4
Object:	HII (SIMBAD class: HIIReg = HII Region)
in source:	NGC 4258
Ref:	=2000MNRAS.318..462D
by	DIAZ A.I. , CASTELLANOS M., TERLEVICH E., GARCIA-VARGAS M.L.
	Mon. Not. R. Astron. Soc., 318, 462-474 (2000)
	Chemical abundances and ionizing clusters of HII regions in the LINER galaxy NGC 4258.
o	Table 6: <[DCT2000] AAN> (Nos GA1-GA4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCT2012]
[DCT2012]	(Davies+Clark+Trombley+, 2012)
Write:	<<[DCT2012] DN-NN>>
N:	14+9
Object:	* (SIMBAD class: Star)
Note:	HST NICMOS imaging and VLT ISAAC spectroscopy of the star clusters Danks 1 and Danks 2.
in source:	Cl Danks 1
in source:	Cl Danks 2
Ref:	=2012MNRAS.419.1871D
by	DAVIES B. , CLARK J.S., TROMBLEY C., FIGER D.F., NAJARRO F., CROWTHER P.A., KUDRITZKI R.-P., THOMPSON M., URQUHART J.S., HINDSON L.
	Mon. Not. R. Astron. Soc., 419, 1871-1886 (2012)
	The G305 star-forming complex: the central star clusters Danks 1 and Danks 2.
o	Table 2: <[DCT2012] DN-NN> (Nos D1-1 to D1-12, D2-1 to D2-9).
Ref:	=2015A&A...575A..10D
by	DE LA FUENTE D. , NAJARRO F., TROMBLEY C., DAVIES B., FIGER D.F.
	Astron. Astrophys., 575A, 10-10 (2015)
	First detections of FS Canis Majoris stars in clusters. Evolutionary state as constrained by coeval massive stars.
o	Figs 7-8: <[DNT2015] McNN-NN> (Nos Mc20-1 to Mc20-17, Mc70-1 to Mc70-14). Table 4: <[DCT2012] DN-NN> (Nos D1-13, D1-14) added. Fig. 15, Table 4: <[DDN2012] NN> (No. 28) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCT2018]
[DCT2018]	(Dreyer+Csizmadia+Titz-Weider+, 2018)= (BEST II)
Write:	<<[DCT2018] F20a NNNNN>> <<[DCT2018] F20a_NNNNN>> (not recognised by Simbad, but found in literature)
N:	2169
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	Berlin Exoplanet Search Telescope II (BEST II) observations of N=2169 variable stars in a target field in the Puppis (Pup) constellation (field F20).
Ref:	=2018AJ....156..204D
by	DREYER C. , CSIZMADIA S., TITZ-WEIDER R., EIGMULLER P., FRUTH T., CABRERA J., ERIKSON A., RAUER H.
	Astron. J., 156, 204-204 (2018)
	The Berlin Exoplanet Search Telescope II catalog of variable stars. III. Census of variable stars in a Puppis field.
o	Table 3: <[DCT2018] F20a NNNNN> N=2169 among (Nos F20a 00022-F20a 31114, F20b 00200-F20b 33916, F20c 00021-F20c 34048, F20d 00027-F20d 30976).
=E=	Catalogue in electronic form as <J/AJ/156/204/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCU2021]
[DCU2021]	(Duarte-Cabral+Colombo+Urquhart+, 2021)
Write:	<<[DCU2021] SDG GLLL.lll+BB.bbbb>> <<[DCU2021] SDGLLL.lll+BB.bbbb>> (not recognised by Simbad, but found in literature)
N:	10663
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	APEX 13CO(2-1) observations of N=10663 molecular clouds in the inner Galaxy, as part of the SEDIGISM (Structure, Excitation, and Dynamics of the Inner Galactic InterStellar Medium) survey. For more information, see http://sedigism.mpifr-bonn.mpg.de
Ref:	=2021MNRAS.500.3027D
by	DUARTE-CABRAL A. , COLOMBO D., URQUHART J.S., GINSBURG A., RUSSEIL D., SCHULLER F., ANDERSON L.D., BARNES P.J., BELTRAN M.T., BEUTHER H., BONTEMPS S., BRONFMAN L., CSENGERI T., DOBBS C.L., EDEN D., GIANNETTI A., KAUFFMANN J., MATTERN M., MEDINA S.-N.X., MENTEN K.M., LEE M.-Y., PETTITT A.R., RIENER M., RIGBY A.J., TRAFICANTE A., VEENA V.S., WIENEN M., WYROWSKI F., AGURTO C., AZAGRA F., CESARONI R., FINGER R., GONZALEZ E., HENNING T., HERNANDEZ A.K., KAINULAINEN J., LEURINI S., LOPEZ S., MAC-AULIFFE F., MAZUMDAR P., MOLINARI S., MOTTE F., MULLER E., NGUYEN-LUONG Q., PARRA R., PEREZ-BEAUPUITS J.-P., MONTENEGRO-MONTES F.M., MOORE T.J.T., RAGAN S.E., SANCHEZ-MONGE A., SANNA A., SCHILKE P., SCHISANO E., SCHNEIDER N., SURI S., TESTI L., TORSTENSSON K., VENEGAS P., WANG K., ZAVAGNO A.
	Mon. Not. R. Astron. Soc., 500, 3027-3049 (2021)
	The SEDIGISM survey: molecular clouds in the inner Galaxy.
o	(Erratum) erratum vol. 513, p.296 (2022)
o	Table A1: <[DCU2021] SDG GLLL.lll+BB.bbbb> N=10663.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DCY96]
[DCY96]	(Drinkwater+Currie+Young+, 1996)
Write:	<<[DCY96] NNN>>
N:	369
Object:	G in ClG (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
in source:	NAME Virgo Cluster
Ref:	=1996MNRAS.279..595D
by	DRINKWATER M.J. , CURRIE M.J., YOUNG C.K., HARDY E., YEARSLEY J.M.
	Mon. Not. R. Astron. Soc., 279, 595-614 (1996)
	Blue compact dwarf galaxies and new velocities in Virgo.
o	Table 9: <[DCY96] NNN> (Nos 1-369)
=E=	Catalogue in electronic form as J/MNRAS/279/595
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DD
DD	(Double Degenerate) (Not yet in Simbad)
*****	Avoid the usage of DD, prefer [H99c]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DD
DD	(Dufour+Duval)
*****	Avoid the usage of DD, prefer [DD75]
Origin	of the Acronym: L (1986A&A...162..180H)
Details on Acronym: DD
DD	(Direct Demodulation)
*****	Avoid the usage of DD, prefer EXO
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Dd
Dd	(Dolidze)= (Do)
Write:	<<PN Dd N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Dd 1 = PN G078.6+05.2 = PK 078+05 1
Ref:	=1971ATsir.629....6D
by	DOLIDZE M.W.
	Astron. Tsirk., 629, 6-7 (1971)
	Emission objects in Cygni.
o	<PN Dd N> (No. 1).
Details on Acronym: [DD2003]
[DD2003]	(Donzelli+Davoust, 2003) (Not yet in Simbad)
Write:	<<[DD2003] HII NN>> <<[DD2003] Knot NN>>
N:	17+10
Object:	HII + Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=17 resolved HII regions in NGC 5666, and N=10 outer knots.
in source:	NGC 5666
Ref:	=2003A&A...409...91D
by	DONZELLI C.J. , DAVOUST E.
	Astron. Astrophys., 409, 91-97 (2003)
	On the nature of the galaxy NGC 5666.
o	Fig.2, Table 3: <[DD2003] HII NN> (Nos 1-17). Fig.3, Table 4: <[DD2003] Knot NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DD2013]
[DD2013]	(Dong+De Robertis, 2013)
Write:	<<[DD2013] W4+N+N NNNNNN>>
N:	2511
Object:	G (SIMBAD class: Galaxy)
Note:	Detection of N=2515 AGN and star-forming galaxy candidates using multi-filter imaging data. Use of CFHTLS data release and SDSS DR7 data.
Ref:	=2013AJ....146...87D
by	DONG X.Y. , DE ROBERTIS M.M.
	Astron. J., 146, 87 (2013)
	Detecting active galactic nuclei using multi-filter imaging data. II. Incorporating artificial neural networks.
o	Table 3: <[DD2013] W4+N+N NNNNNN> N=2515.
=E=	Catalogue in electronic form as J/AJ/146/87
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DD75]
[DD75]	(Dufour+Duval, 1975)= (DD)
Write:	<<[DD75] LMC X-1 NN>> <<[DD75] LMC X-3 NN>>
N:	13+10
Object:	* (SIMBAD class: Star)
Note:	Table I: N=13 stars in the field of LMC X-1 Table III: N=10 stars in the field of LMC X-3 Maps in Figs 1, 3
in source:	Magellanic Clouds:LMC:LMC X-1 = LMC X-1
in source:	Magellanic Clouds:LMC:LMC X-3 = LMC X-3
Ref:	=1975PASP...87..769D
by	DUFOUR R.J. , DUVAL J.E.
	Publ. Astron. Soc. Pac., 87, 769-776 (1975)
	UBV photometry of stars in the direction of three LMC X-ray sources.
o	Table I: <[DD75] LMC X-1 NN> (Nos 1-13). Table III: <[DD75] LMC X-3 NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DD80]
[DD80]	(Davoust+De Vaucouleurs, 1980)= (DV)
Write:	<<[DD80] NNN>> <<[DD80] A>>
N:	133+8
Object:	HII + * (SIMBAD class: HIIReg = HII Region)
Note:	Format 'NNN': 132 HII regions in NGC 7793 No. 133 is added in 1983MNRAS.204..743W ([WS83]) Format 'A': 8 stars (Nos A-H) in NGC 7793
in source:	NGC 7793
Ref:	=1980ApJ...242...30D
by	DAVOUST E. , DE VAUCOULEURS G.
	Astrophys. J., 242, 30-52 (1980)
	Velocity fields in late-type galaxies from Hα Fabry-Perot interferometry. II. Kinematics and dynamics of the Sd spiral NGC 7793.
o	<[DD80] NNN> N=132, <[DD80] A> N=8
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DD88]
[DD88]	(Duric+Dittmar, 1988)
Write:	<<[DD88] NN>>
N:	19
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA 1.4, 4.8, and 15GHz observations of NGC 4736. N=19 compact radio-sources in the near-nuclear region of the galaxy.
in source:	NGC 4736
Ref:	=1988ApJ...332L..67D
by	DURIC N. , DITTMAR M.R.
	Astrophys. J., 332, 67-70 (1988)
	The discovery of a population of compact radio sources in the spiral galaxy NGC 4736.
o	Table 1: <[DD88] NN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DD90]
[DD90]	(Deul+Den Hartog, 1990)= (H)
Write:	<<[DD90] NNN>>
N:	148
Object:	HI Hole (SIMBAD class: PartofG = Part of a Galaxy)
Note:	WSRT HI observations of N=148 HI holes in M 33. Map in Fig.2.
in source:	M 33 = NGC 598
Ref:	=1990A&A...229..362D
by	DEUL E.R. , DEN HARTOG R.H.
	Astron. Astrophys., 229, 362-377 (1990)
	Small-scale structures in the HI distribution of M 33.
o	Table 1: <[DD90] NNN> (Nos 1-148).
=E=	Catalogue in electronic form as J/A+A/229/362
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDA2006]
[DDA2006]	(Diaz+Dottori+Aguero+, 2006) (Not yet in Simbad)
Write:	<<[DDA2006] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	Core (SIMBAD class: denseCore = Dense Core)
Note:	NIR spectroscopy of M83 at the Gemini South 8.1m telescope.
in source:	M 83 = NGC 5236
Ref:	=2006ApJ...652.1122D
by	DIAZ R.J. , DOTTORI H., AGUERO M.P., MEDIAVILLA E., RODRIGUES I., MAST D.
	Astrophys. J., 652, 1122-1128 (2006)
	Hidden trigger for the giant starburst arc in M83?
o	Text: <[DDA2006] J133700.46-295153.6> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDA2010]
[DDA2010]	(Delgado+Djupvik+Alfaro, 2010)
Write:	<<[DDA2010] NNNN>>
N:	1673
Object:	* (SIMBAD class: Star)
Note:	NOT ALFOSC (optical) and NOTCam (NIR) observations of SH 2-284.
in source:	SH 2-284
Ref:	=2010A&A...509A.104D
by	DELGADO A.J. , DJUPVIK A.A., ALFARO E.J.
	Astron. Astrophys., 509A, 104-104 (2010)
	Analysis of the stellar population in the central area of the HII region Sh 2-284.
o	Table 1: <[DDA2010] NNNN> N=1673 among (Nos 2-2634).
=E=	Catalogue in electronic form as J/A+A/509/A104
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DDB
DDB	(D'Odorico+Dopita+Benvenuti)= (D80) = (DDB80)
Write:	<<DDB 1-NN>> <<DDB 2-NN>> <<DDB M 31 NN>> <<DDB NGC NNNN N>> <<DDB IC NNNN N>> <<DDB M 33 NN>>
N:	19+17+19
Object:	Poss. SNR (SIMBAD class: SNRemnant = SuperNova Remnant)
Stat:	is completely incorporated in Simbad
Note:	Table II: SNR candidates in M 31 The authors use the format '1.NN', we use formats '1-NN' and 'M 31 NN, N=19 Table III: SNR candidates in NGC 253, NGC 300, NGC 2403, NGC 6822, IC 1613, IC 342. N=2+7+2+1+1+4 Table IV: SNR candidates in M 33 The authors use the format '2.NN', we use formats '2-NN' and 'M 33 NN, N=19 Identif. charts
in source:	M 31 = NGC 224
in source:	NGC 253
in source:	NGC 300
in source:	NGC 2403
in source:	NGC 6822
in source:	IC 1613
in source:	IC 342
in source:	M 33 = NGC 598
Ref:	=1980A&AS...40...67D
by	D'ODORICO S. , DOPITA M.A., BENVENUTI P.
	Astron. Astrophys., Suppl. Ser., 40, 67-80 (1980)
	A catalogue of supernova remnant candidates in nearby galaxies.
o	Table II: <DDB 1-NN> = <DDB M 31 NN> (Nos 1-19). Table III: <DDB NGC 253 N> (Nos 1-2), <DDB NGC 300 N> (Nos 1-7), <DDB NGC 2403 N> (Nos 1-2), <DDB NGC 6822 N> (No. 1), <DDB IC 1613 N> (No. 1), <DDB IC 342 N> (Nos 1-4). Table IV: <DDB 2-NN> = <DDB M 33 NN> (Nos 1-19)
Origin	of the Acronym: L (1997ApJS..108..261B)
Details on Acronym: [DDB2002]
[DDB2002]	(Demers+Dallaire+Battinelli, 2002)
Write:	<<[DDB2002] NN>>
N:	26
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Note:	2MASS Carbon stars in the Fornax dwarf galaxy.
in source:	NAME Fornax Dwarf Galaxy
Ref:	=2002AJ....123.3428D
by	DEMERS S. , DALLAIRE M., BATTINELLI P.
	Astron. J., 123, 3428-3433 (2002)
	2MASS observations of spectroscopically identified extragalactic C stars.
o	Table 1: <[DDB2002] NN> (Nos 1-26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDB2017]
[DDB2017]	(Dewangan+Devaraj+Baug+, 2017) (Not yet in Simbad)
Write:	<<[DDB2017] NN>> <<[DDB2017] ww-fl>>
N:	39+2
Object:	Clump (SIMBAD class: denseCore = Dense Core)
Note:	N=39 clumps around IRAS 05463+2652. Use of Herschel archival data.
Ref:	=2017ApJ...848...51D
by	DEWANGAN L.K. , DEVARAJ R., BAUG T., OJHA D.K.
	Astrophys. J., 848, 51-51 (2017)
	Embedded filaments in IRAS 05463+2652: early stage of fragmentation and star formation activities.
o	Fig. 1: <[DDB2017] ww-fl> (Nos s-fl, nw-fl). Fig. 4(d), Table 1: <[DDB2017] NN> (Nos 1-39).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DDB80
DDB80	(D'Odorico+Dopita+Benvenuti, 1980)
*****	Avoid the usage of DDB80, prefer DDB
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [DDC93]
[DDC93]	(Dutrey+Duvert+Castets+, 1993)
Write:	<<[DDC93] SN>> <<[DDC93] NN>>
N:	5+20
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Table 1 : large C18O cores, format 'SN', S for Source, N=5 Table 2 : small C18O cores, format 'NN', N=20
in source:	NAME Ori A
Ref:	=1993A&A...270..468D
by	DUTREY A. , DUVERT G., CASTETS A., LANGER W.D., BALLY J., WILSON R.W.
	Astron. Astrophys., 270, 468-476 (1993)
	A multi-transition study of carbon monoxyde in the Orion A molecular cloud.
o	<OMC 3>, Table 1: <[DDC93] SN> N=5, Table 2: <[DDC93] NN> N=20
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDC97]
[DDC97]	(Dantas+De Carvalho+Capelato+, 1997) (Not yet in Simbad)
Write:	<<[DDC97] NNNN>> <<[DDC97] Clump A>>
N:	1421+2
Object:	G + Clump (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	N=1421 G in ACO 3558 Fig.6: N=2 clumps A and B
in source:	ACO 3558
Ref:	=1997ApJ...485..447D
by	DANTAS C.C. , DE CARVALHO R.R., CAPELATO H.V., MAZURE A.
	Astrophys. J., 485, 447-459 (1997)
	Evidence of substructure in the cluster of galaxies A3558.
o	<[DDC97] NNNN> (Nos 1-1421). Fig.6: <[DDC97] Clump A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDC98]
[DDC98]	(Diercks+Deutsch+Castander+, 1998)
Write:	<<[DDC98] N>> <<[DDC98] A>>
N:	5+2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Search for objects near GRB 971214: N=5 calibration stars (Nos 1-5) and N=2 brightest objects (Nos A-B) within 20" of the OT ([INS97] J115626.40+651200.5)
Ref:	=1998ApJ...503L.105D
by	DIERCKS A.H. , DEUTSCH E.W., CASTANDER F.J., CORSON C., GILMORE G., LAMB D.Q., TANVIR N., TURNER E.L., WYSE R.
	Astrophys. J., 503, 105-108 (1998)
	The optical afterglow of GRB 971214: R and J photometry.
o	OT = [INS97] J115626.40+651200.5
o	Table 1, Fig.3: <[DDC98] N> (Nos 1-5), <[DDC98] A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DdDm
DdDm	(Dolidze+Dzimselejsvili)= (DoDz)
Write:	<<PN DdDm N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	DdDm 1 = PN G061.9+41.3 = PK 061+41 1 = PN KO 1
Ref:	=1966ATsir.385....7D
by	DOLIDZE M.V. , JIMSHELEISHVILI G.N.
	Astron. Tsirk., 385, 7-8 (1966)
	New emission object in Hercules.
o	<PN DdDm N> (No. 1).
Details on Acronym: [DDG2006]
[DDG2006]	(De Mello+Dahlen+Gardner+, 2006)
Write:	<<[DDG2006] DDD.ddddddd+DD.ddddddd>>
N:	268
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Note:	WFPC2 U band observations of the GOODS-N and GOODS-S fields.
in source:	NAME GOODS North Field
in source:	NAME GOODS South Field
Ref:	=2006AJ....132.2014D
by	DE MELLO D.F. , DAHLEN T., GARDNER J.P., GROGIN N.A.
	Astron. J., 132, 2014-2023 (2006)
	Near-ultraviolet sources in the Great Observatories Origins Deep Survey fields.
o	Table 1: <[DDG2006] DDD.ddddddd+DD.ddddddd> N=268.
=E=	Catalogue in electronic form as J/AJ/132/2014
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDH2018]
[DDH2018]	(Alla Bonta+Davies+Houghton+, 2018)
Write:	<<[DDH2018] ANN>>
N:	11
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=11 galaxies in the field of Abell 1689. Use of HST ACS, Gemini North GMOS, and VLT FLAMES data. See also [HDD2012] and [DHD2013].
in source:	ACO 1689
Ref:	=2018MNRAS.474..339D
by	DALLA BONTA E. , DAVIES R.L., HOUGHTON R.C.W., D'EUGENIO F., MENDEZ-ABREU J.
	Mon. Not. R. Astron. Soc., 474, 339-387 (2018)
	A photometric analysis of Abell 1689: two-dimensional multistructure decomposition, morphological classification and the Fundamental Plane.
o	Table 2: <[DDH2018] ANN> (Nos A01-A11).
=E=	Catalogue in electronic form as <J/MNRAS/474/339/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DDHW
DDHW	(Danziger+Dopita+Hawarden+Webster)
Write:	<<PN DDHW N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
in source:	NAME Fornax Dwarf Galaxy
Ref:	=1978ApJ...220..458D
by	DANZIGER I.J. , DOPITA M.A., HAWARDEN T.G., WEBSTER B.L.
	Astrophys. J., 220, 458-466 (1978)
	The planetary nebula in the Fornax dwarf galaxy.
o	<PN DDHW N> (No. 1).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [DDJ2017]
[DDJ2017]	(Dupree+Dotter+Johnson+, 2017)
Write:	<<[DDJ2017] NN>>
N:	29
Object:	* (SIMBAD class: Star)
Note:	Magellan/M2FS high-resolution spectroscopic observations of N=29 stars in the LMC cluster NGC 1866.
in source:	NGC 1866
Ref:	=2017ApJ...846L...1D
by	DUPREE A.K. , DOTTER A., JOHNSON C.I., MARINO A.F., MILONE A.P., BAILEY J.I., CRANE J.D., MATEO M., OLSZEWSKI E.W.
	Astrophys. J., 846L, 1-1 (2017)
	NGC 1866: first spectroscopic detection of fast-rotating stars in a young LMC cluster.
o	Table 1: <[DDJ2017] NN> N=29 among (Nos 1-91).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDK2008]
[DDK2008]	(Dedes+Dedes+Kalberla, 2008)
Write:	<<[DDK2008] JHHMMSS.sss+DDMMSS>>
N:	1
Object:	HI Cloud (SIMBAD class: HI = HI (21cm) Source)
Note:	VLA HI observations.
Ref:	=2008A&A...491L..45D
by	DEDES L. , DEDES C., KALBERLA P.M.W.
	Astron. Astrophys., 491L, 45-48 (2008)
	An enigmatic HI cloud.
o	Text: <[DDK2008] JHHMMSS.sss+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDM2000]
[DDM2000]	(Davis+Dent+Matthews+, 2000)
Write:	<<[DDM2000] BN>> <<[DDM2000] RN>> <<[DDM2000] WN>>
N:	3+8
Object:	? (SIMBAD class: PartofCloud = Part of Cloud)
Note:	Outflow from V380 Ori-NE: Fig.1: CO map, (Nos B1, R1-R2) from the Blue and Red lobes. Fig.3: H2 knots north and south of the geometric center of the outflow, (Nos N1-N4, S1-S4).
in source:	NAME V380 Ori-NE
Ref:	=2000MNRAS.318..952D
by	DAVIS C.J. , DENT W.R.F., MATTHEWS H.E., COULSON I.M., McCAUGHREAN M.J.
	Mon. Not. R. Astron. Soc., 318, 952-960 (2000)
	Observations of a curving molecular outflow from V380Ori-NE: further support for prompt entrainment in protostellar outflows.
o	Fig.1: <[DDM2000] AN> (Nos B1, R1-R2). Table 1, Fig.3: <[DDM2000] WN> (Nos N1-N4, S1-S4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDM2001]
[DDM2001]	(Dessauges-Zavadsky+D'odorico+McMahon+, 2001)
Write:	<<[DDM2001] QSO J0307-4945 abs N.NNN>> <<[DDM2001] QSO J0307-4945 abs N.NNNNNN>>
N:	14+26
Object:	Absorber
Note:	UVES observations of the absorber systems in the QSO J0307-4945.
Ref:	=2001A&A...370..426D
by	DESSAUGES-ZAVADSKY M. , D'ODORICO S., McMAHON R.G., MOLARO P., LEDOUX C., PEROUX C., STORRIE-LOMBARDI L.J.
	Astron. Astrophys., 370, 426-435 (2001)
	UVES observations of a damped Lyα system at z_{abs} = 4.466 towards the quasar APM BR J0307-4945.
o	Tables 2, 3: <[DDM2001] QSO J0307-4945 abs N.NNNNNN> N=26. Table 5: <[DDM2001] QSO J0307-4945 abs N.NNN> N=14.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDM2009]
[DDM2009]	(Drake+Djorgovski+Mahabal+, 2009)= (CSS)
Write:	<<[DDM2009] CSSYYMMDD JHHMMSS+DDMMSS>>
N:	61+76+5
Object:	Poss. SN + Poss. CV + Bl? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Catalina Schmidt 0.7m Telescope observations of transients. The first reference is given here. An updated database is available at: http://nesssi.cacr.caltech.edu/catalina/Allns.html
Ref:	=2009ApJ...696..870D
by	DRAKE A.J. , DJORGOVSKI S.G., MAHABAL A., BESHORE E., LARSON S., GRAHAM M.J., WILLIAMS R., CHRISTENSEN E., CATELAN M., BOATTINI A., GIBBS A., HILL R., KOWALSKI R.
	Astrophys. J., 696, 870-884 (2009)
	First results from the Catalina real-time transient survey.
o	Tables 1-3: <[DDM2009] CSSYYMMDD JHHMMSS+DDMMSS> N=61+75+5.
=E=	Catalogue in electronic form as <J/ApJ/696/870/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDM2013]
[DDM2013]	(de la Fuente Marcos+de la Fuente Marcos+Moni Bidin+, 2013)
Write:	<<[DDM2013] NNN>>
N:	356
Object:	* (SIMBAD class: Star)
Note:	CTIO 1m telescope photometry of N=356 stars in the field of the open cluster remnant NGC 1252.
in source:	NGC 1252
Ref:	=2013MNRAS.434..194D
by	DE LA FUENTE MARCOS R. , DE LA FUENTE MARCOS C., MONI BIDIN C., CARRARO G., COSTA E.
	Mon. Not. R. Astron. Soc., 434, 194-208 (2013)
	NGC 1252: a high altitude, metal poor open cluster remnant.
o	<[DDM2013] NNN> (Nos 1-356).
=E=	Catalogue in electronic form as <J/MNRAS/434/194/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDM94]
[DDM94]	(Davis+Dent+Matthews+, 1994) (Not yet in Simbad)
Write:	<<[DDM94] Knot A>> <<[DDM94] Region A>>
N:	25+3
Object:	Knot (SIMBAD class: PartofCloud = Part of Cloud)
Note:	N=25 individual knots in the H2 jet image of LDN 1448, (Nos A-K, M-Z). N=3 regions of emission (Nos J, K, L). See also [BLL93], [E2000].
in source:	LDN 1448
Ref:	=1994MNRAS.266..933D
by	DAVIS C.J. , DENT W.R.F., MATTHEWS H.E., ASPIN C., LIGHTFOOT J.F.
	Mon. Not. R. Astron. Soc., 266, 933-944 (1994)
	Submillimettre and near-infrared observations of L 1448 : a curving H2 jet with multiple bow shocks.
o	Fig.4: <[DDM94] Knot A> (Nos A-K).
Ref:	=1995ApJ...443L..41D
by	DAVIS C.J. , SMITH M.D.
	Astrophys. J., 443, 41-43 (1995)
	Distinction of parallel outflows in L1448 through H2 excitation.
o	Fig.1, Table 1: <[DDM94] Knot A> (Nos T-Z) added. Fig.1: <[DDM94] Region A> (Nos J, K, L).
Ref:	=2000A&A...354..236E
by	EISLOEFFEL J.
	Astron. Astrophys., 354, 236-246 (2000)
	Parsec-scale molecular H_{2} outflows from young stars.
o	Figs 1, 2: <[DDM94] Knot A> (Nos M-S) added. Fig.3: <[E2000] NGC 2071 R> (Nos I-XII), <[E2000] NGC 2071 R A> N=10. Fig.5: <[E2000] NGC 7129 R> (Nos I-IX), <[E2000] NGC 7129 R A> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDN2012]
[DDN2012]	(Davies+De La Fuente+Najarro +, 2012)
Write:	<<[DDN2012] NN>>
N:	12
Object:	* (SIMBAD class: Star)
Note:	HST NICMOS imaging of stars in the candidate star cluster Mercer 81.
in source:	[MCM2005b] 81
Ref:	=2012MNRAS.419.1860D
by	DAVIES B. , DE LA FUENTE D., NAJARRO F., HINTON J.A., TROMBLEY C., FIGER D.F., PUGA E.
	Mon. Not. R. Astron. Soc., 419, 1860-1870 (2012)
	A newly discovered young massive star cluster at the far end of the Galactic Bar.
o	Table 2: <[DDN2012] NN> (Nos 1-10).
Ref:	=2013hsa7.conf..534D
Ref:	=2015A&A...575A..10D
by	DE LA FUENTE D. , NAJARRO F., TROMBLEY C., DAVIES B., FIGER D.F.
	Astron. Astrophys., 575A, 10-10 (2015)
	First detections of FS Canis Majoris stars in clusters. Evolutionary state as constrained by coeval massive stars.
o	Figs 7-8: <[DNT2015] McNN-NN> (Nos Mc20-1 to Mc20-17, Mc70-1 to Mc70-14). Table 4: <[DCT2012] DN-NN> (Nos D1-13, D1-14) added. Fig. 15, Table 4: <[DDN2012] NN> (No. 28) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DDO
DDO	(David Dunlap Obs.)= (Van den Bergh)
Write:	<<DDO NNN>>
N:	243
Object:	Dwarf G (SIMBAD class: Galaxy)
Ref:	=1959PDDO....2..145V
by	VAN DEN BERGH S.
	Publ. David Dunlap Obs., 2, 145-156 (1959)
	A catalogue of dwarf galaxies.
o	Table I: <DDO NNN> (Nos 1-222)
Ref:	=1966AJ.....71..922V
by	VAN DEN BERGH S.
	Astron. J., 71, 922-926 (1966)
	Luminosity classifications of dwarf galaxies.
o	Table II: <DDO NNN> (Nos 223-243)
Details on Acronym: [DDO2006]
[DDO2006]	(Dannerbauer+Daddi+Onodera+, 2006)= (BzK)
Write:	<<[DDO2006] ObjNNNNN>>
N:	23
Object:	G (SIMBAD class: Galaxy)
Note:	IRAM 30m MAMBO 1.2mm observations of five B, z, and K-band preselected vigorous starburst galaxies at z about 2.
Ref:	=2006ApJ...637L...5D
by	DANNERBAUER H. , DADDI E., ONODERA M., KONG X., ROETTGERING H., ARIMOTO N., BRUSA M., CIMATTI A., KURK J., LEHNERT M.D., MIGNOLI M., RENZINI A.
	Astrophys. J., 637, 5-8 (2006)
	MAMBO 1.2 mm observations of BzK-selected star-forming galaxies at z ~ 2.
o	Table 1: <[DDO2006] ObjNNNN> N=5 among (Nos Obj1901 to Obj4415).
Ref:	=2006Natur.442..786G
by	GENZEL R. , TACCONI L.J., EISENHAUER F., FORSTER SCHREIBER N.M., CIMATTI A., DADDI E., BOUCHE N., DAVIES R., LEHNERT M.D., LUTZ D., NESVADBA N., VERMA A., ABUTER R., SHAPIRO K., STERNBERG A., RENZINI A., KONG X., ARIMOTO N., MIGNOLI M.
	Nature, 442, 786-789 (2006)
	The rapid formation of a large rotating disk galaxy three billion years after the Big Bang.
o	Text: <[DDO2006] ObjNNNNN> (No. 15504) added.
Ref:	=2008ApJ...673L..21D
by	DADDI E. , DANNERBAUER H., ELBAZ D., DICKINSON M., MORRISON G., STERN D., RAVINDRANATH S.
	Astrophys. J., 673L, 21-24 (2008)
	Vigorous star formation with low efficiency in massive disk galaxies at z = 1.5.
o	Text: <[DDO2006] ObjNNNNN> (Nos 4171, 21000).
Ref:	=2008ApJ...682..231S
by	SHAPIRO K.L. , GENZEL R., FORSTER SCHREIBER N.M., TACCONI L.J., BOUCHE N., CRESCI G., DAVIES R., EISENHAUER F., JOHANSSON P.H., KRAJNOVIC D., LUTZ D., NAAB T., ARIMOTO N., ARRIBAS S., CIMATTI A., COLINA L., DADDI E., DAIGLE O., ERB D., HERNANDEZ O., KONG X., MIGNOLI M., ONODERA M., RENZINI A., SHAPLEY A., STEIDEL C.
	Astrophys. J., 682, 231-251 (2008)
	Kinemetry of SINS high-redshift star-forming galaxies: distinguishing rotating disks from Major mergers.
o	Galaxy D3a 6397 not identified
o	Table 2: <[DDO2006] ObjNNNNN> (Nos 6004, 12556) added.
Ref:	=2010ApJ...713..686D
by	DADDI E. , BOURNAUD F., WALTER F., DANNERBAUER H., CARILLI C.L., DICKINSON M., ELBAZ D., MORRISON G.E., RIECHERS D., ONODERA M., SALMI F., KRIPS M., STERN D.
	Astrophys. J., 713, 686-707 (2010)
	Very high gas fractions and extended gas reservoirs in z = 1.5 disk galaxies.
o	Table 1: <[DDO2006] ObjNNNNN> (Nos 12591, 16000, 17999, 25536) added.
Ref:	=2011ApJ...729L...4F
by	FERUGLIO C. , DADDI E., FIORE F., ALEXANDER D.M., PICONCELLI E., MALACARIA C.
	Astrophys. J., 729L, 4 (2011)
	Discovery of strong iron kα emitting Compton thick quasars at z = 2.5 and 2.9.
o	Table 2: <[DDO2006] ObjNNNNN> (Nos 4892, 8608) added.
Ref:	=2010ApJ...715..385O
by	ONODERA M. , ARIMOTO N., DADDI E., RENZINI A., KONG X., CIMATTI A., BROADHURST T., ALEXANDER D.M.
	Astrophys. J., 715, 385-405 (2010)
	A wide area survey for high-redshift massive galaxies. II. Near-infrared spectroscopy of BzK-selected massive star-forming galaxies.
o	Table 1: <[KDA2006] D3a NNNNN> N=18 among (Nos 3287-14009). Table 1: <[DDO2006] ObjNNNNN> (Nos 759, 1250, 2079, 3551, 3882, 3977, 4008) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDP2013]
[DDP2013]	(Diaz Tello+Donzelli+Padilla+, 2013)
Write:	<<[DDP2013] SXDF JHHMMSS.s+DDMMSS>> <<[DDP2013] SXDFHHMMSS.s+DDMMSS>> (not recognised by Simbad, but found in literature)
N:	37
Object:	Balmer Break G (SIMBAD class: Galaxy)
Note:	CTIO (u-band photometry), Magellan/IMACS (spectroscopy) and Gemini-South/GMOS (spectroscopy) observations of N=37 Balmer break galaxies.
Ref:	=2013ApJ...771....7D
by	DIAZ TELLO J. , DONZELLI C., PADILLA N., FUJISHIRO N., HANAMI H., YOSHIKAWA T., HATSUKADE B.
	Astrophys. J., 771, 7 (2013)
	Physical properties, star formation, and active galactic nucleus activity in Balmer break galaxies at 0 < z < 1.
o	Table 3: <[DDP2013] SXDF JHHMMSS.s+DDMMSS> N=37.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDP2016]
[DDP2016]	(Diaz Tello+Donzelli+Padilla+, 2016)
Write:	<<[DDP2016] SXDF JHHMMSS.s+DDMMSS>> <<[DDP2016] SXDF HHMMSS.s+DDMMSS>> (not recognised by Simbad, but found in literature)
N:	72
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	CTIO Blanco photometric observations and Magellan IMACS and Gemini-South GMOS spectroscopic observations of N=72 emission line Balmer break galaxies at redshift 0<z<3. See also [DDP2013]
in source:	[DDP2016]
Ref:	=2016A&A...587A.136D
by	DIAZ TELLO J. , DONZELLI C., PADILLA N., AKIYAMA M., FUJISHIRO N., YOSHIKAWA T., HANAMI H.
	Astron. Astrophys., 587A, 136-136 (2016)
	Star formation activity in Balmer break galaxies at z < 1.5.
o	Table A.1: <[DDP2016] SXDF JHHMMSS.s+DDMMSS> N=72.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDR98]
[DDR98]	(Ducourant+Dauphole+Rapaport+, 1998)
Write:	<<[DDR98] NNNNN>> <<[DDR98] PNN>>
N:	36+20
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Tables 3, 4, col(2): N=36+20 stars in the authors' catalogue Table 4, col(1): new presumed nearby candidates (Nos P1-P20)
Ref:	=1998A&A...333..882D
by	DUCOURANT C. , DAUPHOLE B., RAPAPORT M., COLIN J., GEFFERT M.
	Astron. Astrophys., 333, 882-892 (1998)
	Wide field search for nearby faint stars.
o	Table 3: <[DDR98] NNNNN> N=36. Table 4: <[DDR98] NNNNN> = <[DDR98] PNN> (Nos P1-P20) N=20
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDS2009]
[DDS2009]	(Daddi+Dannerbauer+Stern+, 2009)= (VLA)
Write:	<<[DDS2009] VLA NNN>>
N:	3
Object:	(Radio) (SIMBAD class: Radio = Radio Source)
Note:	VLA 1.4GHz observations of the GOODS-N field.
Ref:	=2009ApJ...694.1517D
by	DADDI E. , DANNERBAUER H., STERN D., DICKINSON M., MORRISON G., ELBAZ D., GIAVALISCO M., MANCINI C., POPE A., SPINRAD H.
	Astrophys. J., 694, 1517-1538 (2009)
	Two bright submillimeter galaxies in a z = 4.05 protocluster in GOODS-North, and accurate radio-infrared photometric redshifts.
o	Calibrator source J1044+719 is QSO B1044+719 in Simbad.
o	Table 1: <[PSD2006] GNNN.Na> (Nos GN20.2a and GN20.2b) added. Table 5: <[DDS2009] VLA NNN> (Nos 512, 812, 966).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDS98]
[DDS98]	(Diercks+Deutsch+Stubbs+, 1998)
Write:	<<[DDS98] N>>
N:	5
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	APO 3.5m telescope. N=5 reference stars in the field of GRB 980613.
Ref:	=1998GCN...108....1D
by	DIERCKS A. , DEUTSCH E.W., STUBBS C., VREESWIJK P.M., GALAMA T.J., VAN PARADIJS J., ROBINSON C., KOUVELIOTOU C.
	GRB Coordinates Network, Circular Service, 108, 1-None (1998)
	GRB 980613 optical observations.
o	<[DDS98] N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDT81]
[DDT81]	(Demin+Dibay+Tomov, 1981) (Not yet in Simbad)
Write:	<<[DDT81] NNN>>
N:	105
Object:	Pair of G (SIMBAD class: PairG = Pair of Galaxies)
Ref:	=1981AZh....58..925D
by	DEMIN V.V. , DIBAY E.A., TOMOV A.N.
	Astron. Zh., 58, 925-932 (1981)
	UBV - Photometry of double galaxies. The catalogue.
o	Table 2: <[DDT81] NNN> (Nos 1-105).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDT94]
[DDT94]	(Digel+De Geus+Thaddeus, 1994)= (Digel)
Write:	<<[DDT94] Region NN>> <<[DDT94] Cloud Na>>
N:	63+13
Object:	Region + Cloud (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 1: (Nos 1-63), format 'Region NN'. Tables 2, 3: (Nos 1-8), format 'Cloud Na'.
Ref:	=1994ApJ...422...92D
by	DIGEL S. , DE GEUS E., THADDEUS P.
	Astrophys. J., 422, 92-101 (1994)
	Molecular clouds in the extreme outer galaxy.
o	Table 1: <[DDT94] Region NN> N=63, Tables 2, 3: <[DDT94] Cloud Na> N=13
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDW2012]
[DDW2012]	(Dobbie+Day-Jones+Williams+, 2012)
Write:	<<[DDW2012] NGC 3532-WDC JHHMM+DDMM>> <<[DDW2012] NGC 2287-WDC JHHMM+DDMM>>
N:	11
Object:	Poss. WD (SIMBAD class: WhiteDwarf_Candidate = White Dwarf Candidate)
Note:	ESO 2.2m telescope WFI and VLT FORS2 observations of N=11 white dwarfs in the open clusters NGC 2287 and NGC 3532.
in source:	NGC 3532
in source:	NGC 2287
Ref:	=2012MNRAS.423.2815D
by	DOBBIE P.D. , DAY-JONES A., WILLIAMS K.A., CASEWELL S.L., BURLEIGH M.R., LODIEU N., PARKER Q.A., BAXTER R.
	Mon. Not. R. Astron. Soc., 423, 2815-2828 (2012)
	Further investigation of white dwarfs in the open clusters NGC 2287 and NGC 3532.
o	Table 4: <[DDW2012] NGC 3532-WDC JHHMM+DDMM> N=7, <[DDW2012] NGC 2287-WDC JHHMM+DDMM> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DDW77]
[DDW77]	(Dickel+Dickel+Wilson, 1977)
Write:	<<[DDW77] A>>
N:	4
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	N=4 CO peaks (Nos A-D). Nos A and D are masers. Map in Fig.3
in source:	NGC 6334
Ref:	=1977ApJ...217...56D
by	DICKEL H.R. , DICKEL J.R.
	Astrophys. J., 217, 56-67 (1977)
	The detailed structure of CO in molecular cloud complexes. I. NGC 6334.
o	<[DDW77] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DE95]
[DE95]	(Davis+Eisloffel, 1995)
Write:	<<[DE95] LDN 1157 N>> <<[DE95] LDN 1157 AN>> <<[DE95] VLA 1623 A>> <<[DE95] NGC 6334I N>> <<[DE95] NGC 6334I A>> <<[DE95] NGC 2264G N>> <<[DE95] NGC 2264G AN>> <<[DE95] LDN 1641N N>> <<[DE95] LDN 1641N AN>> <<[DE95] HARO 4-255 A>>
N:	101
Object:	* + knot (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	LDN 1157
in source:	NAME VLA 1623
in source:	NGC 6334:MFSW I = MFSW I
in source:	[MLS88] G
in source:	Orion Nebula:LDN 1641N = LDN 1641N
in source:	Haro 4-255
Ref:	=1995A&A...300..851D
by	DAVIS C.J. , EISLOEFFEL J.
	Astron. Astrophys., 300, 851-869 (1995)
	Near-infrared imaging in H_{2} of molecular (CO) outflows from young stars.
o	(Erratum) erratum in 1996A&A.305.694
o	NGC 2264G = [MLS88] G, VLA N = [GCT94] VLA N, NGC 6334I (I = roman digit) = MFSW I, NGC 6334F = RCM F
o	Table 1, Fig. 1: <[DE95] LDN 1157 N> N=3, <[DE95] LDN 1157 AN> N=18. Table 2, Fig. 4: <[DE95] VLA 1623 A> N=5 Table 3, Fig. 6: <[DE95] NGC 6334I N> N=5, <[DE95] NGC 6334I A> N=4. Table 4, Fig. 8: <[DE95] NGC 2264G N> N=6, <[DE95] NGC 2264G AN> N=26. Table 5, Fig. 10: <[DE95] LDN 1641N N> N=3, <[DE95] LDN 1641N AN> N=13. Fig. 12: <[DE95] HARO 4-255 A> N=8
Ref:	=2006A&A...449.1077C
by	CARATTI O GARATTI A. , GIANNINI T., NISINI B., LORENZETTI D.
	Astron. Astrophys., 449, 1077-1088 (2006)
	H_{2} active jets in the near IR as a probe of protostellar evolution.
o	Fig.11, Table 7: <[DE95] NGC 2264G AN> (Nos I1-I5, H1-H5) added. Fig.12, Table 7: <[CGN2006] VLA 1623 A> (Nos A-D). Fig.12, Table 7: <[GSWC2003] NNa> (Nos 14h, 14i, 17b) added. Fig.17, Table 7: <[NMV2001] Knot A> (Nos N-R) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DEA2008]
[DEA2008]	(Dye+Eales+Aretxaga+, 2008)
Write:	<<[DEA2008] Lock850.NNNb>>
N:	13
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Subaru SuprimeCam secondary counterparts of SHADES sources (SCUBA Half Degree Extragalactic Survey) in the Lockman Hole. Use of UKIRT UKIDSS data. See also [CCM2006].
in source:	NAME Lockman Hole
Ref:	=2008MNRAS.386.1107D
by	DYE S. , EALES S.A., ARETXAGA I., SERJEANT S., DUNLOP J.S., BABBEDGE T.S.R., CHAPMAN S.C., CIRASUOLO M., CLEMENTS D.L., COPPIN K.E.K., DUNNE L., EGAMI E., FARRAH D., IVISON R.J., VAN KAMPEN E., POPE A., PRIDDEY R., RIEKE G.H., SCHAEL A.M., SCOTT D., SIMPSON C., TAKAGI T., TAKATA T., VACCARI M.
	Mon. Not. R. Astron. Soc., 386, 1107-1130 (2008)
	The SCUBA HAlf Degree Extragalactic Survey (SHADES) - VII. Optical/IR photometry and stellar masses of submillimetre galaxies.
o	Table 2: <[DEA2008] Lock850.NNNb> N=13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DEB2010]
[DEB2010]	(Dunham+Evans+Bourke+, 2010)
Write:	<<[DEB2010] L673-7-IRS>>
N:	1
Object:	Protostar (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	Spitzer and CSO SHARC-II observations of the dense core [LM99] L673-7.
in source:	[LM99] L673-7
Ref:	=2010ApJ...721..995D
by	DUNHAM M.M. , EVANS N.J., BOURKE T.L., MYERS P.C., HUARD T.L., STUTZ A.M.
	Astrophys. J., 721, 995-1013 (2010)
	The Spitzer c2d survey of nearby dense cores. IX. Discovery of a very low luminosity object driving a molecular outflow in the dense core L673-7.
o	<[DEB2010] L673-7-IRS>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DEE99]
[DEE99]	(Dinshaw+Evans+Epps+, 1999) (Not yet in Simbad)
Write:	<<[DEE99] NN>>
N:	12
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
in source:	NGC 6090
Ref:	=1999ApJ...525..702D
by	DINSHAW N. , EVANS A.S., EPPS H., SCOVILLE N.Z., RIEKE M.
	Astrophys. J., 525, 702-708 (1999)
	NICMOS observations of interaction-triggered star formation in the luminous infrared galaxy NGC 6090.
o	Table 1: <[DEE99] NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DEEP-GSS
DEEP-GSS	(DEEP, Groth Strip Survey)= (Groth) = (GSS)
Write:	<<DEEP-GSS FFN-xxyya>>
Object:	G (SIMBAD class: Galaxy)
Note:	HST WFPC2 parameters of galaxies in the 'Groth Strip' (28 overlapping fields). In the format 'FF' is the GSS field, 'N' is the WFPC2 chip, and 'xx' and 'yy' are the object coordinates on the chips in units of 10 pixels. A letter 'a' is added when a group of objects are close enough to have the same primary ID. See [HI2001] and [ISF2002], 2 first designations using the DEEP-GSS ID.
Ref:	=2002ApJS..142....1S
by	SIMARD L. , WILLMER C.N.A., VOGT N.P., SARAJEDINI V.L., PHILLIPS A.C., WEINER B.J., KOO D.C., IM M., ILLINGWORTH G.D., FABER S.M.
	Astrophys. J., Suppl. Ser., 142, 1-33 (2002)
	The DEEP Groth Strip Survey. II. Hubble Space Telescope structural parameters of galaxies in the Groth Strip.
o	Tables 2, 3: <DEEP-GSS FFC-xxyya> N=7451.
Ref:	=2005ApJ...620..595W
by	WEINER B.J. , PHILLIPS A.C., FABER S.M., WILLMER C.N.A., VOGT N.P., SIMARD L., GEBHARDT K., IM M., KOO D.C., SARAJEDINI V.L., WU K.L., FORBES D.A., GRONWALL C., GROTH E.J., ILLINGWORTH G.D., KRON R.G., RHODES J., SZALAY A.S., TAKAMIYA M.
	Astrophys. J., 620, 595-617 (2005)
	The DEEP Groth Strip galaxy redshift survey. III. Redshift catalog and properties of galaxies.
o	Table 1: <DEEP-GSS FFC-xxyya> N=71 added.
=E=	Catalogue in electronic form as J/ApJS/142/1
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DEEP2
DEEP2	(Deep Extragalactic Evolutionary Probe 2)
Write:	<<DEEP2 JHHMMSS.s+DDMMSS>>
N:	about 32780
Object:	G (SIMBAD class: Galaxy)
Note:	The recently completed DEEP2 Galaxy Redshift Survey gives the most detailed view of the z∼1 Universe currently available. Using the DEIMOS spectrograph on the Keck II telescope, DEEP2 obtained spectra for about 50000 galaxies out to z=1.4. The survey covers about 3 square degrees of sky, split over four separate fields. One of the fields is the Extended Groth Strip, which has IAU acronym designation EGSD2 and format JHHMMSS.ss+DDMMSS.s. DEEP2 will be used for the galaxies in the remaining three fields. More information about the DEEP2 survey is at http://deep.berkeley.edu/.
Ref:	=2009ApJ...698..956C
by	COMERFORD J.M. , GERKE B.F., NEWMAN J.A., DAVIS M., YAN R., COOPER M.C., FABER S.M., KOO D.C., COIL A.L., ROSARIO D.J., DUTTON A.A.
	Astrophys. J., 698, 956-965 (2009)
	Inspiralling supermassive black holes: a new signpost for galaxy mergers.
o	Table 1: <EGSD2 JHHMMSS.s+DDMMSS> N=20, <DEEP2 JHHMMSS.s+DDMMSS> N=12.
=E=	Catalogue in electronic form as <II/301/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: DEEP2-GRS
DEEP2-GRS	(DEEP2, Galaxy Redshift Survey)
Write:	<<DEEP2-GRS NNNNNNNN>>
Object:	G (SIMBAD class: Galaxy)
Note:	DEEP2-GRS uses DEIMOS on Keck II telescope to survey optical galaxies at z about 1. The first paper citing DEEP2-GRS objects reports Keck II NIRSPEC spectroscopy of galaxies from the DEEP2 galaxy redshift survey.
Ref:	=2005ApJ...635.1006S
by	SHAPLEY A.E. , COIL A.L., MA C.-P., BUNDY K.
	Astrophys. J., 635, 1006-1021 (2005)
	Chemical abundances of DEEP2 star-forming galaxies at z~1.0-1.5.
o	Table 1: <DEEP2-GRS NNNNNNNN> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Dehnen
Dehnen	(Dehnen)
*****	Avoid the usage of Dehnen, prefer [D98b]
Origin	of the Acronym: L (2016BaltA..25..377M)
Details on Acronym: DeHt
DeHt	(Dengel+Hartl+)
*****	Avoid the usage of DeHt, prefer DHW
Origin	of the Acronym: L = Found in the literature
Details on Acronym: DeHt
DeHt	(Dengel+Hartl+)= (DHW)
Write:	<<PN DeHt N>>
N:	5
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	See also 'DHW 1' one possible PN, in 1979MitAG..45..182D
Ref:	=1980A&A....85..356D
by	DENGEL J. , HARTL H., WEINBERGER R.
	Astron. Astrophys., 85, 356-358 (1980)
	A search for planetary nebulae on the "POSS".
o	<PN DeHt N> (Nos 1-5).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Dejc
Dejc	(Russian transliteration of DEUTSCH)
*****	Avoid the usage of Dejc, prefer Deutsch
Details on Acronym: Deje
Deje	(Russian transliteration of DEUTSCH)
*****	Avoid the usage of Deje, prefer Deutsch
Details on Acronym: Delalande
Delalande	(Delalande)
*****	Avoid the usage of Delalande, prefer Lal
Details on Acronym: DELS
DELS	(DESI Legacy imaging Survey)
Write:	<<DELS NNNNNNNNNNNNNNNN>>
Object:	(Opt) (SIMBAD class: Optical = Optical Source)
Note:	The catalog object number provided by the DESI Legacy Imaging Surveys is the combination the following fields: release,brickid,objid. For more information, visit: https://www.legacysurvey.org/
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DELS
DELS	(DESI Legacy imaging survey)
Write:	<<DELS JHHMMSS.ss+DDMMSS.s>> <<DELS JHHMM+DDMM>> (not recognised by Simbad, but found in literature)
N:	?
Object:	(Opt) (SIMBAD class: Optical = Optical Source)
Note:	DECaLS, together with the g, r-bands Beijing-Arizona Sky Survey (BASS, Zou et al. 2017PASP..129f4101Z) and the Mayall z-band Legacy Survey (MzLS) provide imaging to support target selection for the Dark Energy Spectroscopic Instrument (DESI), and are collectively referred to as the DESI Legacy imaging survey (DELS). Only the first reference citing DELS objects is listed here.
Ref:	=2017ApJ...839...27W
by	WANG F. , FAN X., YANG J., WU X.-B., YANG Q., BIAN F., McGREER I.D., LI J.-T., LI Z., DING J., DEY A., DYE S., FINDLAY J.R., GREEN R., JAMES D., JIANG L., LANG D., LAWRENCE A., MYERS A.D., ROSS N.P., SCHLEGEL D.J., SHANKS T.
	Astrophys. J., 839, 27-27 (2017)
	First discoveries of z > 6 quasars with the DECam Legacy Survey and UKIRT Hemisphere Survey.
o	Table 3: <DELS JHHMMSS.ss+DDMMSS.s> N=3. Table 4: <[WFY2017] JHHMMSS.ss+DDMMSS.s> N=44.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DEM
DEM	(Davies+Elliot+Meaburn)= (DEML) = (DEM-LMC) = (LMC-DEM) = (DEMS) = (DEM-SMC) = (SMC-DEM)
Write:	<<DEM L NNNa>> <<DEM S NNN>>
N:	329+172
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	In the format, the letter 'L' stands for LMC, the letter 'S' for SMC. Identif. charts.
in source:	Magellanic Clouds:LMC = LMC
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1976MmRAS..81...89D
by	DAVIES R.D. , ELLIOTT K.H., MEABURN J.
	Mem. R. Astron. Soc., 81, 89-128 (1976)
	The nebular complexes of the Large and Small Magellanic Clouds.
o	DEM
o	Table II: <DEM L NNNa> (Nos 1-329) N=357. Table III: <DEM S NNN> (Nos 1-167).
Ref:	=1986MNRAS.223..317M
by	MEABURN J.
	Mon. Not. R. Astron. Soc., 223, 317-321 (1986)
	Young-star formation in the Magellanic H I bridge.
o	Table 1: <DEM S NNN> (Nos 168-172)
=E=	Catalogue in electronic form as VII/232
Details on Acronym: DEM-LMC
DEM-LMC	(Davies+Elliot+Meaburn, LMC)
*****	Avoid the usage of DEM-LMC, prefer DEM
Details on Acronym: DEM-SMC
DEM-SMC	(Davies+Elliot+Meaburn, SMC)
*****	Avoid the usage of DEM-SMC, prefer DEM
Details on Acronym: [DEM2009]
[DEM2009]	(Donnarumma+Ettori+Meneghetti+, 2009)
Write:	<<[DEM2009] ANN>>
N:	6
Object:	Arc (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Analysis of HST WFPC2 images of the MS2137.3-2353 lensing system. See also [[FLH92].
in source:	1E 2137.0-2353
Ref:	=2009MNRAS.398..438D
by	DONNARUMMA A. , ETTORI S., MENEGHETTI M., MOSCARDINI L.
	Mon. Not. R. Astron. Soc., 398, 438-450 (2009)
	X-ray and strong lensing mass estimate of MS2137.3-2353.
o	Fig. 6: Galaxy 01 is [FLH92] G7 in Simbad.
o	Fig. 6, Text: <[DEM2009] ANN> (Nos A01-A02, A3-A4, B1-B2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DEM2011]
[DEM2011]	(Donnarumma+Ettori+Meneghetti+, 2011)
Write:	<<[DEM2011] BCG>> <<[DEM2011] N>> <<[DEM2011] A>> <<[DEM2011] AN>>
N:	1+7+4+14
Object:	Brightest Cluster Galaxy + G + Grav. lensed image of a G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations of ACO 611.
in source:	ACO 611
Ref:	=2011A&A...528A..73D
by	DONNARUMMA A. , ETTORI S., MENEGHETTI M., GAVAZZI R., FORT B., MOSCARDINI L., ROMANO A., FU L., GIORDANO F., RADOVICH M., MAOLI R., SCARAMELLA R., RICHARD J.
	Astron. Astrophys., 528A, 73-73 (2011)
	Abell 611. II. X-ray and strong lensing analyses.
o	Fig. 5, Table 4: <[DEM2011] BCG> N=1, <[DEM2011] N> (Nos 1-7). Fig. 5: <[DEM2011] A> (Nos A-D), <[DEM2011] AN> (Nos A1-A3, B1-B5, C1-C2, D1-D4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DEM94]
[DEM94]	(Dalton+Efstathiou+Maddox+, 1994)
Write:	<<[DEM94] HHMMSS.s+DDMMSS>>
N:	228
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=23 clusters. Table 4: Cluster catalogue constructed from the APM Galaxy Survey, N=189 See also APMCC
Ref:	=1994MNRAS.269..151D
by	DALTON G.B. , EFSTATHIOU G., MADDOX S.J., SUTHERLAND W.J.
	Mon. Not. R. Astron. Soc., 269, 151-165 (1994)
	The APM galaxy survey. IV. Redshifts of rich clusters of galaxies.
o	(Erratum) erratum vol. 273 p.528
o	Table 3: <APMGS HHMMSS.ss-DDMMSS.s> N=365. Tables 1, 2, 4: <[DEM94] HHMMSS.s-DDMMSS> N=228
=E=	Catalogue in electronic form as J/MNRAS/269/151
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Demers
Demers	(Demers+)
*****	Avoid the usage of Demers, prefer [DKG90]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: DEML
DEML	(Davies+Elliot+Meaburn, LMC)
*****	Avoid the usage of DEML, prefer DEM
Details on Acronym: DEMS
DEMS	(Davies+Elliot+Meaburn, SMC)
*****	Avoid the usage of DEMS, prefer DEM
Details on Acronym: DEN
DEN	(Deep Near-Infrared Survey, Provisory designation)
*****	Avoid the usage of DEN, prefer DENIS-P
Origin	of the Acronym: L (2001ApJ...548..908L)
Details on Acronym: DENIS
DENIS	(Deep Near-Infrared Survey)= (DBD)
Write:	<<DENIS JHHMMSS.s+DDMMSS>>
N:	355220325
Object:	(Near IR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	This catalogue of the Southern sky is the latest incremental release of the DENIS project. It consists of a set of 355220325 point sources detected by the DENIS survey in 3662 strips (covering each 30 degrees in declination and 12 arcmin in right ascension).
Ref:	=1999A&A...349..236E
by	EPCHTEIN N. , DEUL E., DERRIERE S., BORSENBERGER J., EGRET D., SIMON G., ALARD C., BALAZS L.G., DE BATZ B., CIONI M.-R., COPET E., DENNEFELD M., FORVEILLE T., FOUQUE P., GARZON F., HABING H.J., HOLL A., HRON J., KIMESWENGER S., LACOMBE F., LE BERTRE T., LOUP C., MAMON G.A., OMONT A., PATUREL G., PERSI P., ROBIN A.C., ROUAN D., TIPHENE D., VAUGLIN I., WAGNER S.J.
	Astron. Astrophys., 349, 236-242 (1999)
	A preliminary database of DENIS point sources.
o	<DENIS JHHMMSS.s-DDMMSS> N=355220325.
Ref:	=2005yCat.2263....0T
by	THE DENIS CONSORTIUM
	yCat, 2263, 0 (2005)
	The DENIS database, 3rd Release.
=E=	Catalogue in electronic form as B/denis
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DENIS-P
DENIS-P	(Deep Near-Infrared Survey, Provisory designation)= (DNS) = (DENIS) = (DEN)
Write:	<<DENIS JHHMM.m+DDMMA>> <<DENIS JHHMMSS.s+DDMMSS>>
Object:	(Near IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	First refs with DENIS-P objects
Ref:	=1997A&A...327L..25D
by	DELFOSSE X. , TINNEY C.G., FORVEILLE T., EPCHTEIN N., BERTIN E., BORSENBERGER J., COPET E., DE BATZ B., FOUQUE P., KIMESWENGER S., LE BERTRE T., LACOMBE F., ROUAN D., TIPHENE D.
	Astron. Astrophys., 327, 25-28 (1997)
	Field brown dwarfs found by DENIS.
o	p. L26 2MASP J0345 = 2MASP J0345432+254023.
o	Table 1: <DENIS-P JHHMM.m+DDMM> N=3.
Ref:	=1999Sci...283.1718M
by	MARTIN E.L. , BRANDNER W., BASRI G.
	Science, 283, 1718-1720 (1999)
	A search for companions to nearby brown dwarfs: the binary DENIS-P J1228.2-1547.
o	<DENIS-P J1228.2-1547A> (Nos A-B).
Ref:	=1999A&A...348..755O
by	OMONT A. , GANESH S., ALARD C., BLOMMAERT J.A.D.L., CAILLAUD B., COPET E., FOUQUE P., GILMORE G., OJHA D., SCHULTHEIS M., SIMON G., BERTOU X., BORSENBERGER J., EPCHTEIN N., GLASS I., GUGLIELMO F., GROENEWEGEN M.A.T., HABING H.J., KIMESWENGER S., MORRIS M., PRICE S.D., ROBIN A., UNAVANE M., WYSE R.
	Astron. Astrophys., 348, 755-767 (1999)
	ISOGAL-DENIS detection of red giants with weak mass loss in the Galactic Bulge.
o	Table 2: <[OGA99] NNN> N=62 among (Nos 14-799) = <ISOGAL-P JHHMMSS.s+DDMMSS> N=62 = <DENIS-P JHHMMSS.s+DDMMSS> N=61.
Ref:	=2000JApA...21...77O
by	OJHA D.K. , OMONT A., GANESH S., SIMON G., SCHULTHEIS M.
	J. Astrophys. Astron., 21, 77-90 (2000)
	Stellar sources in the ISOGAL inner Galactic Bulge field (l = 0°, b = -1°).
o	Table 2: <[OOG2000] NNN> N=27 among (Nos 29-568) = <ISOGAL-P JHHMMSS.s+DDMMSS> N=27 = <DENIS-P JHHMMSS.s+DDMMSS> N=27.
Ref:	=2000A&A...363...62R
by	ROUSSEAU J. , PATUREL G., VAUGLIN I., SCHROEDER A., DE BATZ B., BORSENBERGER J., EPCHTEIN N., FOUQUE P., KIMESWENGER S., LACOMBE F., LE BERTRE T., MAMON G., ROUAN D., SIMON G., TIPHENE D.
	Astron. Astrophys., 363, 62-68 (2000)
	Some noteworthy DENIS galaxies near the galactic plane.
o	Tables 1, 2: : <[RPV2000] NN> (Nos 1-37). Table A1: <DENIS-P JHHMMSS.s+DDMMSS> N=1212.
Ref:	=2002A&A...387....1V
by	VAUGLIN I. , ROUSSEAU J., PATUREL G., BORSENBERGER J., EPCHTEIN N., FOUQUE P., KIMESWENGER S., LE BERTRE T., MAMON G.A.
	Astron. Astrophys., 387, 1-7 (2002)
	Serendipitous detection of galaxies behind the Milky Way from the DENIS survey.
o	Table 1: <[VRP2002] JHHMMSS.s+DDMMSS> N=2027 = <DENIS-P JHHMMSS.s+DDMMSS> N=2027.
Ref:	=2003A&A...405....1P
by	PATUREL G. , PETIT C., ROUSSEAU J., VAUGLIN I.
	Astron. Astrophys., 405, 1-3 (2003)
	The provisional DENIS I-band catalog of galaxies revisited.
o	<DENIS-P JHHMMSS.s+DDMMSS> N=42258.
=E=	Catalogue in electronic form as J/A+A/363/62
=E=	Catalogue in electronic form as J/A+A/387/1
=E=	Catalogue in electronic form as VII/234
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DENIS-RED
DENIS-RED	(Deep Near-Infrared Survey, Rapid Extraction from DENIS) (Not yet in Simbad)
*****	Avoid the usage of DENIS-RED, prefer DENISP
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DENISP
DENISP	(Deep Near-Infrared Survey, Provisory)= (DENIS-RED) (Not yet in Simbad)
Write:	<<DENISP G JHHMMSSs+DDMMSS>>
N:	20260
Object:	G (SIMBAD class: Galaxy)
Note:	REDCAT is the release of the provisional extragalactic catalogue constructed from the "Deep Near Infrared Southern Sky Survey" (DENIS). This catalogue contains 20260 galaxies with coordinates and I-band photometry (magnitude, diameter, axis ratio, position angle and a parameter related to the morphological type).
Ref:	=1999A&AS..135..133V
by	VAUGLIN I. , PATUREL G., BORSENBERGER J., FOUQUE P., EPCHTEIN N., KIMESWENGER S., TIPHENE D., LANOIX P., COURTOIS H.
	Astron. Astrophys., Suppl. Ser., 135, 133-144 (1999)
	First DENIS I-band extragalactic catalog.
o	Catalogue: <DENISP G JHHMMSSs+DDMMSS> N=20260.
=E=	Catalogue in electronic form as J/A+AS/135/133
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DER94]
[DER94]	(Davis+Eisloffel+Ray, 1994)
Write:	<<[DER94] HH 1-2 NN>>
N:	11
Object:	Knot (SIMBAD class: HerbigHaroObj = Herbig-Haro Object)
Stat:	is completely incorporated in Simbad
Note:	Knots in HH 1-2 complex. See also [O95].
in source:	NAME HH 1-2
Ref:	=1994ApJ...426L..93D
by	DAVIS C.J. , EISLOEFFEL J., RAY T.P.
	Astrophys. J., 426, 93-95 (1994)
	Near-infrared imaging of HH 1/2 in shocked molecular hydrogen and [FeII].
o	The other knots in HH NNN objects have a format 'HH NNNA' or 'HH NNNAN'.
o	<HH NNN> (No. 147). Fig.1: <[DER94] HH 1-2 N> (Nos 1-8).
Ref:	=2000A&A...359.1147E
by	EISLOEFFEL J. , SMITH M.D., DAVIS C.J.
	Astron. Astrophys., 359, 1147-1161 (2000)
	Spectroscopy of molecular hydrogen in outflows from young stars.
o	Figs 2, 3, Table 2: <[DER94] HH 1-2 NN> (Nos 9-10) added. Fig5, Table 3: <[MDR98] a> (Nos i-k) added.
Ref:	=2000MNRAS.318..747D
by	DAVIS C.J. , SMITH M.D., EISLOEFFEL J.
	Mon. Not. R. Astron. Soc., 318, 747-752 (2000)
	New, high-resolution, near-infrared observations of HH1.
o	Fig.1: <[DER94] HH 1-2 NN> (No. 11) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DER97]
[DER97]	(Davis+Eisloffel+Ray+, 1997) (Not yet in Simbad)
Write:	<<[DER97] A>>
N:	5
Object:	HH (SIMBAD class: HerbigHaroObj = Herbig-Haro Object)
Note:	Fig.1, 4: HH objects associated with the NE-SW outflow of RNO 15 FIR.
Ref:	=1997A&A...324.1013D
by	DAVIS C.J. , EISLOEFFEL J., RAY T.P., JENNESS T.
	Astron. Astrophys., 324, 1013-1019 (1997)
	Prompt entrainment in the variable molecular jet from RNO 15-FIR.
o	Fig. 1, 4: <[DER97] A> (Nos A-E)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DES
DES	(Dark Energy Survey)
Write:	<<DES JHHMMSS.ss+DDMMSS.s>>
N:	about 600000000
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	The Dark Energy Survey (DES) is an optical survey in the g, r, i, z, Y filter bands that will be conducted on the CTIO Blanco 4m telescope with a new 3 sq deg imager (the Dark Energy Camera, or DECam) during the 2011-2016 time frame. It will cover 5000 sq deg in the Southern Galactic Cap down to 26.1, 25.6, 25.8, 25.3, 23.3 in g, r, i, z, Y (5-sigma limits for point sources). For more information, please see: http://www.darkenergysurvey.org/ http://cosmology.uiuc.edu/DES/ http://www.ctio.noao.edu/decam/
Ref:	=2018ApJS..239...18A
by	ABBOTT T.M.C. , ABDALLA F.B., ALLAM S., AMARA A., ANNIS J., ASOREY J., AVILA S., BALLESTER O., BANERJI M., BARKHOUSE W., BARUAH L., BAUMER M., BECHTOL K., BECKER M.R., BENOIT-LEVY A., BERNSTEIN G.M., BERTIN E., BLAZEK J., BOCQUET S., BROOKS D., BROUT D., BUCKLEY-GEER E., BURKE D.L., BUSTI V., CAMPISANO R., CARDIEL-SAS L., CARNERO ROSELL A., CARRASCO KIND M., CARRETERO J., CASTANDER F.J., CAWTHON R., CHANG C., CHEN X., CONSELICE C., COSTA G., CROCCE M., CUNHA C.E., D'ANDREA C.B., DA COSTA L.N., DAS R., DAUES G., DAVIS T.M., DAVIS C., DE VICENTE J., DEPOY D.L., DEROSE J., DESAI S., DIEHL H.T., DIETRICH J.P., DODELSON S., DOEL P., DRLICA-WAGNER A., EIFLER T.F., ELLIOTT A.E., EVRARD A.E., FARAHI A., NETO A.F., FERNANDEZ E., FINLEY D.A., FLAUGHER B., FOLEY R.J., FOSALBA P., FRIEDEL D.N., FRIEMAN J., GARCIA-BELLIDO J., GAZTANAGA E., GERDES D.W., GIANNANTONIO T., GILL M.S.S., GLAZEBROOK K., GOLDSTEIN D.A., GOWER M., GRUEN D., GRUENDL R.A., GSCHWEND J., GUPTA R.R., GUTIERREZ G., HAMILTON S., HARTLEY W.G., HINTON S.R., HISLOP J.M., HOLLOWOOD D., HONSCHEID K., HOYLE B., HUTERER D., JAIN B., JAMES D.J., JELTEMA T., JOHNSON M.W.G., JOHNSON M.D., KACPRZAK T., KENT S., KHULLAR G., KLEIN M., KOVACS A., KOZIOL A.M.G., KRAUSE E., KREMIN A., KRON R., KUEHN K., KUHLMANN S., KUROPATKIN N., LAHAV O., LASKER J., LI T.S., LI R.T., LIDDLE A.R., LIMA M., LIN H., LOPEZ-REYES P., MacCRANN N., MAIA M.A.G., MALONEY J.D., MANERA M., MARCH M., MARRINER J., MARSHALL J.L., MARTINI P., McCLINTOCK T., McKAY T., McMAHON R.G., MELCHIOR P., MENANTEAU F., MILLER C.J., MIQUEL R., MOHR J.J., MORGANSON E., MOULD J., NEILSEN E., NICHOL R.C., NOGUEIRA F., NORD B., NUGENT P., NUNES L., OGANDO R.L.C., OLD L., PACE A.B., PALMESE A., PAZ-CHINCHON F., PEIRIS H.V., PERCIVAL W.J., PETRAVICK D., PLAZAS A.A., POH J., POND C., PORREDON A., PUJOL A., REFREGIER A., REIL K., RICKER P.M., ROLLINS R.P., ROMER A.K., ROODMAN A., ROONEY P., ROSS A.J., RYKOFF E.S., SAKO M., SANCHEZ M.L., SANCHEZ E., SANTIAGO B., SARO A., SCARPINE V., SCOLNIC D., SERRANO S., SEVILLA-NOARBE I., SHELDON E., SHIPP N., SILVEIRA M.L., SMITH M., SMITH R.C., SMITH J.A., SOARES-SANTOS M., SOBREIRA F., SONG J., STEBBINS A., SUCHYTA E., SULLIVAN M., SWANSON M.E.C., TARLE G., THALER J., THOMAS D., THOMAS R.C., TROXEL M.A., TUCKER D.L., VIKRAM V., VIVAS A.K., WALKER A.R., WECHSLER R.H., WELLER J., WESTER W., WOLF R.C., WU H., YANNY B., ZENTENO A., ZHANG Y., ZUNTZ J., (The DES Collaboration), JUNEAU S., FITZPATRICK M., NIKUTTA R., NIDEVER D., OLSEN K., SCOTT A., (The NOAO Data Lab)
	Astrophys. J., Suppl. Ser., 239, 18-18 (2018)
	The Dark Energy Survey: data release 1.
o	<DES JHHMMSS.ss+DDMMSS.s> N=399263026.
Ref:	=2021ApJS..255...20A
by	ABBOTT T.M.C. , ADAMOW M., AGUENA M., ALLAM S., AMON A., ANNIS J., AVILA S., BACON D., BANERJI M., BECHTOL K., BECKER M.R., BERNSTEIN G.M., BERTIN E., BHARGAVA S., BRIDLE S.L., BROOKS D., BURKE D.L., CARNERO ROSELL A., CARRASCO KIND M., CARRETERO J., CASTANDER F.J., CAWTHON R., CHANG C., CHOI A., CONSELICE C., COSTANZI M., CROCCE M., DA COSTA L.N., DAVIS T.M., DE VICENTE J., DEROSE J., DESAI S., DIEHL H.T., DIETRICH J.P., DRLICA-WAGNER A., ECKERT K., ELVIN-POOLE J., EVERETT S., EVRARD A.E., FERRERO I., FERTE A., FLAUGHER B., FOSALBA P., FRIEDEL D., FRIEMAN J., GARCIA-BELLIDO J., GAZTANAGA E., GELMAN L., GERDES D.W., GIANNANTONIO T., GILL M.S.S., GRUEN D., GRUENDL R.A., GSCHWEND J., GUTIERREZ G., HARTLEY W.G., HINTON S.R., HOLLOWOOD D.L., HONSCHEID K., HUTERER D., JAMES D.J., JELTEMA T., JOHNSON M.D., KENT S., KRON R., KUEHN K., KUROPATKIN N., LAHAV O., LI T.S., LIDMAN C., LIN H., MacCRANN N., MAIA M.A.G., MANNING T.A., MALONEY J.D., MARCH M., MARSHALL J.L., MARTINI P., MELCHIOR P., MENANTEAU F., MIQUEL R., MORGAN R., MYLES J., NEILSEN E., OGANDO R.L.C., PALMESE A., PAZ-CHINCHON F., PETRAVICK D., PIERES A., PLAZAS A.A., POND C., RODRIGUEZ-MONROY M., ROMER A.K., ROODMAN A., RYKOFF E.S., SAKO M., SANCHEZ E., SANTIAGO B., SCARPINE V., SERRANO S., SEVILLA-NOARBE I., SMITH J.A., SMITH M., SOARES-SANTOS M., SUCHYTA E., SWANSON M.E.C., TARLE G., THOMAS D., TO C., TREMBLAY P.E., TROXEL M.A., TUCKER D.L., TURNER D.J., VARGA T.N., WALKER A.R., WECHSLER R.H., WELLER J., WESTER W., WILKINSON R.D., YANNY B., ZHANG Y., NIKUTTA R., FITZPATRICK M., JACQUES A., SCOTT A., OLSEN K., HUANG L., HERRERA D., JUNEAU S., NIDEVER D., WEAVER B.A., ADEAN C., CORREIA V., DE FREITAS M., FREITAS F.N., SINGULANI C., VILA-VERDE G., (The Linea Science Server)
	Astrophys. J., Suppl. Ser., 255, 20-20 (2021)
	The Dark Energy Survey data release 2.
o	<DES JHHMMSS.ss+DDMMSS.s> N about 688000000.
=E=	Catalogue in electronic form as <II/357/>
=E=	Catalogue in electronic form as <II/371/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: DES
DES	(Dark Energy Survey)
Write:	<<DES JHHMM.m+DDMM>> <<DES JHHMM+DDMM>>
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Additional formats related to the Dark Energy Survey (DES) and used in the literature. Only one reference per format is listed here.
Ref:	=2015ApJ...807...50B
by	BECHTOL K. , DRLICA-WAGNER A., BALBINOT E., PIERES A., SIMON J.D., YANNY B., SANTIAGO B., WECHSLER R.H., FRIEMAN J., WALKER A.R., WILLIAMS P., ROZO E., RYKOFF E.S., QUEIROZ A., LUQUE E., BENOIT-LEVY A., TUCKER D., SEVILLA I., GRUENDL R.A., DA COSTA L.N., FAUSTI NETO A., MAIA M.A.G., ABBOTT T., ALLAM S., ARMSTRONG R., BAUER A.H., BERNSTEIN G.M., BERNSTEIN R.A., BERTIN E., BROOKS D., BUCKLEY-GEER E., BURKE D.L., CARNERO ROSELL A., CASTANDER F.J., COVARRUBIAS R., D'ANDREA C.B., DEPOY D.L., DESAI S., DIEHL H.T., EIFLER T.F., ESTRADA J., EVRARD A.E., FERNANDEZ E., FINLEY D.A., FLAUGHER B., GAZTANAGA E., GERDES D., GIRARDI L., GLADDERS M., GRUEN D., GUTIERREZ G., HAO J., HONSCHEID K., JAIN B., JAMES D., KENT S., KRON R., KUEHN K., KUROPATKIN N., LAHAV O., LI T.S., LIN H., MAKLER M., MARCH M., MARSHALL J., MARTINI P., MERRITT K.W., MILLER C., MIQUEL R., MOHR J., NEILSEN E., NICHOL R., NORD B., OGANDO R., PEOPLES J., PETRAVICK D., PLAZAS A.A., ROMER A.K., ROODMAN A., SAKO M., SANCHEZ E., SCARPINE V., SCHUBNELL M., SMITH R.C., SOARES-SANTOS M., SOBREIRA F., SUCHYTA E., SWANSON M.E.C., TARLE G., THALER J., THOMAS D., WESTER W., ZUNTZ J., (The DES Collaboration)
	Astrophys. J., 807, 50 (2015)
	Eight new Milky Way companions discovered in first-year dark energy survey data.
o	Table 1: <[BDB2015] DES JHHMM.m+DDMM> N=8.
Ref:	=2015ApJ...813..109D
by	DRLICA-WAGNER A. , BECHTOL K., RYKOFF E.S., LUQUE E., QUEIROZ A., MAO Y.-Y., WECHSLER R.H., SIMON J.D., SANTIAGO B., YANNY B., BALBINOT E., DODELSON S., NETO A.F., JAMES D.J., LI T.S., MAIA M.A.G., MARSHALL J.L., PIERES A., STRINGER K., WALKER A.R., ABBOTT T.M.C., ABDALLA F.B., ALLAM S., BENOIT-LEVY A., BERNSTEIN G.M., BERTIN E., BROOKS D., BUCKLEY-GEER E., BURKE D.L., CARNERO ROSELL A., CARRASCO KIND M., CARRETERO J., CROCCE M., DA COSTA L.N., DESAI S., DIEHL H.T., DIETRICH J.P., DOEL P., EIFLER T.F., EVRARD A.E., FINLEY D.A., FLAUGHER B., FOSALBA P., FRIEMAN J., GAZTANAGA E., GERDES D.W., GRUEN D., GRUENDL R.A., GUTIERREZ G., HONSCHEID K., KUEHN K., KUROPATKIN N., LAHAV O., MARTINI P., MIQUEL R., NORD B., OGANDO R., PLAZAS A.A., REIL K., ROODMAN A., SAKO M., SANCHEZ E., SCARPINE V., SCHUBNELL M., SEVILLA-NOARBE I., SMITH R.C., SOARES-SANTOS M., SOBREIRA F., SUCHYTA E., SWANSON M.E.C., TARLE G., TUCKER D., VIKRAM V., WESTER W., ZHANG Y., ZUNTZ J., (The DES Collaboration)
	Astrophys. J., 813, 109 (2015)
	Eight ultra-faint galaxy candidates discovered in year two of the dark energy survey.
o	Tables 1-2: <[DBR2015] DES JHHMM+DDMM> N=8. <NAME Grus II> = <NAME Gru II>. <NAME Tucana R > = <NAME Tuc R> (Nos III-V) added. <NAME Columba I> = <NAME Col I>. <NAME Reticulum III> = <NAME Ret III>. <NAME Indus II> = <NAME Ind II>. <NAME Cetus II> = <NAME Cet II>.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: DES
DES	(Dark Energy Survey)
Write:	<<DES YYANaaaa>>
Object:	Poss. SN (SIMBAD class: Supernova_Candidate = SuperNova Candidate)
Note:	SN candidates discovered by the Dark Energy Survey. The adopted naming convention is the following: DES{season}{field}{index} where {season} is the year pertaining to the beginning of each observing season, {field} denotes one of the ten SN search fields (E1, E2, S1, S2, X1, X2, X3, C1, C2, C3) in Elais-S1 (E), Stripe 82 (S), XMM-LSS (X) and CDF-S (C), and {index} is one or more lower-case letters starting from a-z, then aa-az, and so on. The DES SN Survey strategy is described in Bernstein et al. 2012ApJ...753..152B. Only the first reference with SN candidates is given here.
Ref:	=2012ATel.4668....1A
by	ABBOTT T. , ABDALLA F., ACHITOUV I., AHN E., ALDERING G., ALLAM S., ALONSO D., AMARA A., ANNIS J., ANTONIK M., ARAGON-SALAMANCA A., ARMSTRONG R., ASHALL C., ASOREY J., BACON D., BALBINOT E., BANERJI M., BARBARY K., BARKHOUSE W., BARUAH L., BAUER A., BECHTOL K., BECKER M., BENDER R., BENOIST C., BENOIT-LEVY A., BERNARDI M., BERNSTEIN G., BERNSTEIN J.P., BERNSTEIN R., BERTIN E., BEYNON E., BHATTACHARYA S., BIESIADZINSKI T., BISWAS R., BLAKE C., BLOOM J.S., BOCQUET S., BRANDT C., BRIDLE S., BROOKS D., BROWN P.J., BRUNNER R., BUCKLEY-GEER E., BURKE D., BURKERT A., BUSHA M., CAMPA J., CAMPBELL H., CANE R., CAPOZZI D., CARLSTROM J., CARNERO ROSELL A., CAROLLO M., CARRASCO-KIND M., CARRETERO J., CARTER M., CASAS R., CASTANDER F.J., CHEN Y., CHIU I., CHUE C., CLAMPITT J., CLERKIN L., COHN J., COLLESS M., COPELAND E., COVARRUBIAS R.A., CRITTENDEN R., CROCCE M., CUNHA C., DA COSTA L., D'ANDREA C., DAS S., DAS R., DAVIS T.M., DEB S., DEPOY D., DERYLO G., DESAI S., DE SIMONI F., DEVLIN M., DIEHL H.T., DIETRICH J., DODELSON S., DOEL P., DOLAG K., EFSTATHIOU G., EIFLER T., ERICKSON B., ERIKSEN M., ESTRADA J., ETHERINGTON J., EVRARD A., FARRENS S., FAUSTI A., FERNANDEZ E., FERREIRA P.C., FINLEY D., FISCHER J.A., FLAUGHER B., FOSALBA P., FRIEMAN J., FURLANETTO C., GARCIA-BELLIDO J., GAZTANAGA E., GELMAN M., GERDES D., GIANNANTONIO T., GILHOOL S., GILL M., GLADDERS M., GLADNEY L., GLAZEBROOK K., GRAY M., GRUEN D., GRUENDL R., GUPTA R., GUTIERREZ G., HABIB S., HALL E., HANSEN S., HAO J., HEITMANN K., HELSBY J., HENDERSON R., HENNIG C., HIGH W., HIRSCH M., HOFFMANN K., HOLHJEM K., HONSCHEID K., HOST O., HOYLE B., HU W., HUFF E., HUTERER D., JAIN B., JAMES D., JARVIS M., JARVIS M.J., JELTEMA T., JOHNSON M., JOUVEL S., KACPRZAK T., KARLINER I., KATSAROS J., KENT S., KESSLER R., KIM A., KIM-VY T., KING L., KIRK D., KOCHANEK C., KOPP M., KOPPENHOEFER J., KOVACS E., KRAUSE E., KRAVTSOV A., KRON R., KUEHN K., KUEMMEL M., KUHLMANN S., KUNDER A., KUROPATKIN N., KWAN J., LAHAV O., LEISTEDT B., LEVI M., LEWIS P., LIDDLE A., LIDMAN C., LILLY S., LIN H., LIU J., LOPEZ-ARENILLAS C., LORENZON W., LOVERDE M., MA Z., MAARTENS R., MACCRANN N., MACRI L., MAIA M., MAKLER M., MANERA M., MARASTON C., MARCH M., MARKOVIC K., MARRINER J., MARSHALL J., MARSHALL S., MARTINI P., MARTI P., MAYERS J., MCKAY T., MCMAHON R., MELCHIOR P., MERRITT K.W., MERSON A., MILLER C., MIQUEL R., MOHR J., MOORE T., MORTONSON M., MOSHER J., MOULD J., MUKHERJEE P., NEILSEN E., NGEOW C., NICHOL R., NIDEVER D., NORD B., NUGENT P., OGANDO R., OLD L., OLSEN J., OSTROVSKI F., PAECH K., PAPADOPOULOS A., PAPOVICH C., PATTON K., PEACOCK J., PELLEGRINI P.S.S., PEOPLES J., PERCIVAL W., PERLMUTTER S., PETRAVICK D., PLAZAS A., PONCE R., POOLE G., POPE A., REFREGIER A., REYES R., RICKER P., ROE N., ROMER K., ROODMAN A., ROONEY P., ROSS A., ROWE B., ROZO E., RYKOFF E., SABIU C., SAGLIA R., SAKO M., SANCHEZ A., SANCHEZ C., SANCHEZ E., SANCHEZ J., SANTIAGO B., SARO A., SCARPINE V., SCHINDLER R., SCHMIDT B.P., SCHMITT R.L., SCHUBNELL M., SEITZ S., SENGER R., SEVILLA I., SHARP R., SHELDON E., SHETH R., SMITH R.C., SMITH M., SNIGULA J., SOARES-SANTOS M., SOBREIRA F., SONG J., SOUMAGNAC M., SPINKA H., STEBBINS A., STOUGHTON C., SUCHYTA E., SUHADA R., SULLIVAN M., SUN F., SUNTZEFF N., SUTHERLAND W., SWANSON M.E.C., SYPNIEWSKI A.J., SZEPIETOWSKI R., TALAGA R., TARLE G., TARRANT E., BALAN S.T., THALER J., THOMAS D., THOMAS R.C., TUCKER D., UDDIN S.A., URAL S., VIKRAM V., VOIGT L., WALKER A.R., WALKER T., WECHSLER R., WEINBERG D., WELLER J., WESTER W., WETZSTEIN M., WHITE M., WILCOX H., WILMAN D., YANNY B., YOUNG J., ZABLOCKI A., ZENTENO A., ZHANG Y., ZUNTZ J.
	ATel, 4668, 1 (2012)
	First SN discoveries from the Dark Energy Survey.
o	<DES YYANaaa> N=3.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DES
DES	(Deeply Embedded Source)
*****	Avoid the usage of DES, prefer [YIN2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DESC
DESC	(Deeply Embedded Sub Cluster)
*****	Avoid the usage of DESC, prefer [LML2004]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DESI
DESI	(Dark Energy Spectroscopic Instrument)
Write:	<<DESI JDDD.dddd+DD.dddd>>
N:	about 60000000 (SIMBAD class: Optical = Optical Source)
Note:	DESI is a cosmological survey with the goal of measuring optical spectra and redshifts for roughly 40 million extragalactic redshifts and another roughly 15-20 million stars. Website: https://www.desi.lbl.gov/ Experiment Design Paper: https://ui.adsabs.harvard.edu/abs/2016arXiv161100036D/abstract
Notes:	None of the existing publications use this naming scheme, but very few name individual objects. The ones that do use the unique TARGETID given to a DESI target, which is sufficient but less human readable.
Auth.:	Anthony Kremin Lawrence Berkeley National Laboratory
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: DETWC
DETWC	(De Gioia-Eastwood+Throop+Walker+Cudworth)
Write:	<<DETWC Tr NN JHHMMSS.s+DDMMSS>>
N:	280+560
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	Cl Trumpler 14
in source:	Cl Trumpler 16
Ref:	=2001ApJ...549..578D
by	DEGIOIA-EASTWOOD K. , THROOP H., WALKER G., CUDWORTH K.M.
	Astrophys. J., 549, 578-589 (2001)
	The star formation history of Trumpler 14 and Trumpler 16.
o	Table 1: <DETWC Tr 14 JHHMMSS.s+DDMMSS> N=280. Table 2: <DETWC Tr 16 JHHMMSS.s+DDMMSS> N=560.
=E=	Catalogue in electronic form as J/ApJ/549/578
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Deutsch
Deutsch	(Deutsch)= (Dejc) = (Deje)
Write:	<<NAME Deutsch's object ->>
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Ref:	=1963ATsir.259....1D
by	DEUTSCH A.N.
	Astron. Tsirk., 259, 1-2 (1963)
	New intergalactic globular cluster?
o	<NAME Deutsch's object>
Details on Acronym: deV
deV	(De Vaucouleurs+)
*****	Avoid the usage of deV, prefer [DPD83]
Origin	of the Acronym: L (2002ApJ...572..838B)
Details on Acronym: DeV
DeV	(De Vaucouleurs)
*****	Avoid the usage of DeV, prefer DV
Origin	of the Acronym: L (1988SSRv...48....1R)
Details on Acronym: Dev G
Dev G	(De Vaucouleurs, G)
*****	Avoid the usage of Dev G, prefer DV
Origin	of the Acronym: L = Found in the literature
Details on Acronym: DF
DF	(Deep Field) (Not yet in Simbad)
*****	Avoid the usage of DF, prefer DSS
Origin	of the Acronym: L (1987AJ.....93..805W)
Details on Acronym: DF
DF	(Diffuse Feature)
*****	Avoid the usage of DF, prefer [DV78]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DF
DF	(Dark Filament)
*****	Avoid the usage of DF, prefer [THP2002]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 2dF
2dF	(2dF survey)
*****	Avoid the usage of 2dF, prefer [EET2007]
Origin	of the Acronym: L (2007A&A...462..397E)
Details on Acronym: [DF2014]
[DF2014]	(Di Teodoro+Fraternali, 2014)
Write:	<<[DF2014] NN>>
N:	10
Object:	G (SIMBAD class: Galaxy)
Note:	HI observations of N=10 nearby spiral galaxies. Use of the Westerbork Hi survey of Irregular and Spiral galaxies Project (WHISP).
Ref:	=2014A&A...567A..68D
by	DI TEODORO E.M. , FRATERNALI F.
	Astron. Astrophys., 567A, 68-68 (2014)
	Gas accretion from minor mergers in local spiral galaxies.
o	Table 1: <[DF2014] NN> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DFBS
DFBS	(Digitized First Byurakan Survey)
Write:	<<DFBS JHHMMSS.ss+DDMMSS.s>>
N:	13 (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	The First Byurakan Survey (FBS) is an objective-prism spectral survey that covers the largest area to date. It is performed with the Byurakan Observatory Schmidt telescope, which covers about 17 000 sq. deg.
Ref:	=2012A&A...544A..95G
by	GIGOYAN K.S. , RUSSEIL D., MICKAELIAN A.M., SARKISSIAN A., AVTANDILYAN M.G.
	Astron. Astrophys., 544A, 95-95 (2012)
	New carbon stars found in the Digitized First Byurakan Survey.
o	Table 1:<DFBS JHHMMSS.ss+DDMMSS.s> N=13
=E=	Catalogue in electronic form as VI/116
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DFE2004]
[DFE2004]	(D'Elia+Fiore+Elvis+, 2004)
Write:	<<[DFE2004] JHHMMSS+DDMMSS>> <<[DFE2004] A>>
N:	6
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Chandra observation of X-ray sources around 3C 295 Cluster: N=6 galaxies close to extended X-ray sources.
in source:	NAME 3C 295 Cluster
Ref:	=2004A&A...422...11D
by	D'ELIA V. , FIORE F., ELVIS M., CAPPI M., MATHUR S., MAZZOTTA P., FALCO E., COCCHIA F.
	Astron. Astrophys., 422, 11-21 (2004)
	The faint X-ray source population near 3C 295.
o	MRC 1138-206 is a misprint for MRC 1138-262. Fig.1, text: extended source = EQ J141137+521835 in SIMBAD
o	Table 1, Fig.2: <[DFE2004] A> (Nos A-F). Text, Fig.1: <[DFE2004] JHHMMSS+DDMMSS> N=1.
=E=	Catalogue in electronic form as <=>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFF2007]
[DFF2007]	(Dettbarn+Fuchs+Flynn+, 2007)
Write:	<<[DFF2007] SN>>
N:	3
Object:	Stellar Stream (SIMBAD class: Association = Association of Stars)
Note:	N=3 star streams in the Galactic halo.
Ref:	=2007A&A...474..857D
by	DETTBARN C. , FUCHS B., FLYNN C., WILLIAMS M.
	Astron. Astrophys., 474, 857-861 (2007)
	Signatures of star streams in the phase space distribution of nearby halo stars.
o	Table 1: <[DFF2007] SN> (Nos S1-S3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFF2020]
[DFF2020]	(Dutta+Fumagalli+Fossati+, 2020)
Write:	<<[DFF2020] JHHMMSS.ss+DDMMSS.s>>
N:	228
Object:	G (SIMBAD class: Galaxy)
Note:	N=228 galaxies in 28 quasar fields from the MUSE Analysis of Gas around Galaxies (MAGG) survey. Use of archival data from VLT UVES and X-SHOOTER, Keck HIRES and ESI, Magellan MIKE. See also [LFF2020].
Ref:	=2020MNRAS.499.5022D
by	DUTTA R. , FUMAGALLI M., FOSSATI M., LOFTHOUSE E.K., PROCHASKA J.X., ARRIGONI BATTAIA F., BIELBY R.M., CANTALUPO S., COOKE R.J., MURPHY M.T., O'MEARA J.M.
	Mon. Not. R. Astron. Soc., 499, 5022-5046 (2020)
	MUSE Analysis of Gas around Galaxies (MAGG) - II: metal-enriched halo gas around z ~ 1 galaxies.
o	Table S2: <[DFF2020] JHHMMSS.ss+DDMMSS.s> N=228.
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [DFG2002]
[DFG2002]	(Dallacasa+Fanti+Giacintucci+, 2002) (Not yet in Simbad)
Write:	<<[DFG2002] HHMM+DDdA WN>> <<[DFG2002] HHMM+DDdA C>> <<[DFG2002] HHMM+DDdA CeN>>
N:	54
Object:	Component (SIMBAD class: Radio = Radio Source)
Note:	Radio components of 18 B3 sources. See also [FPD2001b], [DTF2002], [ODF2004].
Ref:	=2002A&A...389..126D
by	DALLACASA D. , FANTI C., GIACINTUCCI S., STANGHELLINI C., FANTI R., GREGORINI L., VIGOTTI M.
	Astron. Astrophys., 389, 126-142 (2002)
	The B3-VLA CSS sample. III. EVN & MERLIN images at 18 cm.
o	Figs, Table 2: <[DFG2002] HHMM+DDdA WN>, <[DFG2002] HHMM+DDdA C>, <[DFG2002] HHMM+DDdA CeN>, N=54.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFG98]
[DFG98]	(Durret+Felenbok+Gerbal+, 1998)
Write:	<<[DFG98] N>>
N:	4
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Combined analysis of ROSAT PSPC and optical data Table 1: N=4 X-ray sources in ACO 85 See also [SDG98] and [DFL98]
in source:	ACO 85
Ref:	=1998A&A...335...41D
by	DURRET F. , FORMAN W., GERBAL D., JONES C., VIKHLININ A.
	Astron. Astrophys., 335, 41-48 (1998)
	The rich cluster of galaxies ABCG 85. III. Analyzing the ABCG 85/87/89 complex.
o	Sample regions ANN (Table 2) not in SIMBAD
o	Table 1: <[DFG98] N> (Nos 1-4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 2dFGRS
2dFGRS	(2dF Galaxy Redshift Survey)
Write:	<<2dFGRS AAWFFFANNN>>
N:	about 250000
Object:	G (SIMBAD class: Galaxy)
Note:	The '2dFGRS' source catalogue is a revised and extended version of the APM catalogue. It contains about 250000 objects. First references with 2dFGRS objects.
Ref:	=1999PASA...16..247S
by	SADLER E.M. , McINTYRE V.J., JACKSON C.A., CANNON R.D.
	Publications - Astron. Soc. Australia, 16, 247-256 (1999)
	Radio sources in the 2dF Galaxy Redshift Survey. I. Radio source populations.
o	Table 2: <2dFGRS AAWFFFANNN> N=89.
Ref:	=2001MNRAS.328.1039C
by	COLLESS M. , DALTON G., MADDOX S., SUTHERLAND W., NORBERG P., COLE S., BLAND-HAWTHORN J., BRIDGES T., CANNON R., COLLINS C., COUCH W., CROSS N., DEELEY K., DE PROPRIS R., DRIVER S.P., EFSTATHIOU G., ELLIS R.S., FRENK C.S., GLAZEBROOK K., JACKSON C., LAHAV O., LEWIS I., LUMSDEN S., MADGWICK D., PEACOCK J.A., PETERSON B.A., PRICE I., SEABORNE M., TAYLOR K.
	Mon. Not. R. Astron. Soc., 328, 1039-1063 (2001)
	The 2dF Galaxy Redshift Survey: spectra and redshifts.
o	Catalogue: <2dFGRS AAWFFFANNN> N=102426.
Ref:	=2002MNRAS.329..227S
by	SADLER E.M. , JACKSON C.A., CANNON R.D., McINTYRE V.J., MURPHY T., BLAND-HAWTHORN J., BRIDGES T., COLE S., COLLESS M., COLLINS C., COUCH W., DALTON G., DE PROPRIS R., DRIVER S.P., EFSTATHIOU G., ELLIS R.S., FRENK C.S., GLAZEBROOK K., LAHAV O., LEWIS I., LUMSDEN S., MADDOX S., MADGWICK D., NORBERG P., PEACOCK J.A., PETERSON B.A., SUTHERLAND W., TAYLOR K.
	Mon. Not. R. Astron. Soc., 329, 227-245 (2002)
	Radio sources in the 2dF Galaxy Redshift Survey - II. Local radio luminosity functions for AGN and star-forming galaxies at 1.4 GHz.
o	Table 1: <2dFGRS AAWFFFANNN> N=912.
Ref:	=2002MNRAS.334..209M
by	MADGWICK D.S. , HEWETT P.C., MORTLOCK D.J., LAHAV O.
	Mon. Not. R. Astron. Soc., 334, 209-218 (2002)
	Spectroscopic detection of quasars in the 2dF Galaxy Redshift Survey.
o	Table 1: <2dFGRS AAWFFFANNN> N=55.
=E=	Catalogue in electronic form as VII/226
=E=	Catalogue in electronic form as VII/250
=E=	Catalogue in electronic form as J/MNRAS/329/227
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 2dFGRS
2dFGRS	(2dF Galaxy Redshift Survey)
*****	Avoid the usage of 2dFGRS, prefer [EET2007]
Origin	of the Acronym: L (2007A&A...462..397E)
Details on Acronym: 2dFGRS
2dFGRS	(2dF Galaxy Redshift Survey)
*****	Avoid the usage of 2dFGRS, prefer [TEE2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 6dFGS
6dFGS	(6-degree Field Galaxy Survey)
Write:	<<6dFGS gJHHMMSS.s+DDMMSS>> <<6dFGS JHHMMSSs+DDMMSS>> (not recognised by Simbad, but found in literature)
N:	124647
Object:	G (SIMBAD class: Galaxy)
Note:	Galaxies from the 6dFGS. The authors used a format gHHMMSS+DDMMSS where the letter g stands for galaxy, then 2000 coordinates, so the letter 'J' is added. 2009MNRAS.399..683J: The 6dF Galaxy Survey Redshift Catalogue Data Release 3 (final release).
Ref:	=2009MNRAS.399..683J
by	JONES D.H. , READ M.A., SAUNDERS W., COLLESS M., JARRETT T., PARKER Q.A., FAIRALL A.P., MAUCH T., SADLER E.M., WATSON F.G., BURTON D., CAMPBELL L.A., CASS P., CROOM S.M., DAWE J., FIEGERT K., FRANKCOMBE L., HARTLEY M., HUCHRA J., JAMES D., KIRBY E., LAHAV O., LUCEY J., MAMON G.A., MOORE L., PETERSON B.A., PRIOR S., PROUST D., RUSSELL K., SAFOURIS V., WAKAMATSU K.-I., WESTRA E., WILLIAMS M.
	Mon. Not. R. Astron. Soc., 399, 683-698 (2009)
	The 6dF galaxy survey: final redshift release (DR3) and southern large-scale structures.
o	<6dFGS gJHHMMSS.s+DDMMSS> N=124647.
=E=	Catalogue in electronic form as VII/259/6dfgs
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DFI99]
[DFI99]	(Deguchi+Fujii+Izumiura+, 1999) (Not yet in Simbad)
Write:	<<[DFI99] IRAS 18019-1822 A>> <<[DFI99] IRAS 18465-0717 A>> <<[DFI99] IRAS 18019-1822 N>> <<[DFI99] IRAS 18465-0717 N>>
N:	2+2+4+2
Object:	Maser + (IR) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 1: Radio components A and B to each IRAS, corresponding to pairs of stars, each with an SiO maser source. Table 4: Possible (IR) counterparts of IRAS.
in source:	IRAS 18019-1822
in source:	IRAS 18465-0717
Ref:	=1999PASJ...51..355D
by	DEGUCHI S. , FUJII T., IZUMIURA H., MATSUMOTO S., NAKADA Y., WOOD P.R., YAMAMURA I.
	Publ. Astron. Soc. Jap., 51, 355-361 (1999)
	Apparent double SiO maser sources.
o	Table 1: <[DFI99] IRAS 18019-1822 A> (Nos A-B), <[DFI99] IRAS 18465-0717 A> (Nos A-B). Table 4: <[DFI99] IRAS 18019-1822 N> (Nos 1-4), <[DFI99] IRAS 18465-0717 N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFJ2001]
[DFJ2001]	(Donnelly+Forman+Jones+, 2001)
Write:	<<[DFJ2001] JHHMMSS.s+DDMMSS>> <<[DFJ2001] ANNNN WW>>
N:	72+68+157+6
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	ROSAT and ASCA observations of ACO 3528, ACO 1750, ACO 3395.
in source:	ACO 3528
in source:	ACO 1750
in source:	ACO 3395
Ref:	=2001ApJ...562..254D
by	DONNELLY R.H. , FORMAN W., JONES C., QUINTANA H., RAMIREZ A., CHURAZOV E., GILFANOV M.
	Astrophys. J., 562, 254-265 (2001)
	Merging binary clusters.
o	Table 2: <[DFJ2001] ANNNN WW> N=6. Tables 3, 4, 5: <[DFJ2001] JHHMMSS.s+DDMMSS> N=72+68+157.
=E=	Catalogue in electronic form as J/ApJ/562/254
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFJ2007]
[DFJ2007]	(de Ugarte Postigo+Fatkhullin+Johannesson+, 2007)
Write:	<<[DFJ2007] NN>>
N:	12
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Optical photometric calibration with the 1.54m Danish telescope at La Silla and the 1.5m telescope at Sierra Nevada Observatory. N=12 calibration stars in the field of GRB 050408.
Ref:	=2007A&A...462L..57D
by	DE UGARTE POSTIGO A. , FATKHULLIN T.A., JOHANNESSON G., GOROSABEL J., SOKOLOV V.V., CASTRO-TIRADO A.J., BALEGA Y.Y., SPIRIDONOVA O.I., JELINEK M., GUZIY S., PEREZ-RAMIREZ D., HJORTH J., LAURSEN P., BERSIER D., PANDEY S.B., BREMER M., MONFARDINI A., HUANG K.Y., URATA Y., IP W.H., TAMAGAWA T., KINOSHITA D., MIZUNO T., ARAI Y., YAMAGISHI H., SOYANO T., USUI F., TASHIRO M., ABE K., ONDA K., ASLAN Z., KHAMITOV I., OZISIK T., KIZILOGLU U., BIKMAEV I., SAKHIBULLIN N., BURENIN R., PAVLINSKY M., SUNYAEV R., BHATTACHARYA D., KAMBLE A.P., ISHWARA CHANDRA C.H., TRUSHKIN S.A.
	Astron. Astrophys., 462L, 57-60 (2007)
	Extensive multiband study of the X-ray rich GRB 050408. A likely off-axis event with an intense energy injection.
o	Fig.A1, Table A1: <[DFJ2007] NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFJ99]
[DFJ99]	(David+Forman+Jones, 1999)
Write:	<<[DFJ99] ACO NNNNW>>
N:	6
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	N=6 subclusters in ACO galaxy clusters. Use of ROSAT PSPC observations.
Ref:	=1999ApJ...519..533D
by	DAVID L.P. , FORMAN W., JONES C.
	Astrophys. J., 519, 533-548 (1999)
	ROSAT PSPC observations of the richest (R≥2) ACO clusters.
o	Table 1: <[DFJ99] ACO NNNNW> (Nos 625W, 625E, 1758S, 1758N, 2246W, 2246E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFK2001]
[DFK2001]	(Djorgovski+Frail+Kulkarni+, 2001)= (VLA)
Write:	<<[DFK2001] VLA JHHMMSS.s+DDMMSS>> <<[DFK2001] Galaxy A>> <<[DFK2001] Star N>>
N:	1+3+1+1
Object:	(Rad) + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Study of the field around GRB 970828. N=1 VLA radio transient, associated with GRB 970828. N=3+1 galaxies, and N=1 star. See also [KES97].
Ref:	=2001ApJ...562..654D
by	DJORGOVSKI S.G. , FRAIL D.A., KULKARNI S.R., BLOOM J.S., ODEWAHN S.C., DIERCKS A.
	Astrophys. J., 562, 654-663 (2001)
	The afterglow and the host galaxy of the dark burst GRB 970828.
o	<[DFK2001] VLA JHHMMSS.s+DDMMSS> N=1. Fig3: <[DFK2001] Galaxy A> (Nos A-C, G), <[DFK2001] Star N> (No. 1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFK2009]
[DFK2009]	(Davies+Figer+Kudritzki+, 2009) (Not yet in Simbad)
Write:	<<[DFK2009] NNa>> <<[DFK2009] Aa>>
N:	29
Object:	* (SIMBAD class: Star)
Note:	Keck NIRC2 imaging and Keck NIRSPEC spectroscopy of the cluster associated with the magnetar SGR 1900+14. See also [VLH96], [VHL2000].
in source:	NAME Sgr 1900+14
in source:	NAME Sgr 1900+14 Star Cluster
Ref:	=2009ApJ...707..844D
by	DAVIES B. , FIGER D.F., KUDRITZKI R.-P., TROMBLEY C., KOUVELIOTOU C., WACHTER S.
	Astrophys. J., 707, 844-851 (2009)
	The progenitor mass of the magnetar SGR1900+14.
o	Fig. 1: <[DFK2009] NNa> (Nos 1a-1d, 4a-4b, 5a-5b, 6a-6b, 7a-7d, 8a-8b, 9a-9c, 10a-10b), <[DFK2009] Aa> (Nos Ba-Bd, Ca-Cb). Fig. 2, Table 2: <[DFK2009] NN> (Nos 13, 15).
o	Cl 1813-13 is a misprint for Cl 1813-18 which is object [MFD2008] Stellar Cluster in SIMBAD.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFL98]
[DFL98]	(Durret+Felenbok+Lobo+, 1998)
Write:	<<[DFL98] NNN>> <<[DFL98] Star NN>>
N:	551+39
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table 4: N=550 galaxies in ACO 85 (Nos 330 and 331 are the same galaxy). Table 3: N=39 * misclassifed as galaxies See also [SDG98] and [DFG98]
in source:	ACO 85
Ref:	=1998A&AS..129..281D
by	DURRET F. , FELENBOK P., LOBO C., SLEZAK E.
	Astron. Astrophys., Suppl. Ser., 129, 281-288 (1998)
	A catalogue of velocities in the cluster of galaxies Abell 85.
o	See also 1998A&AS..128...67S.
o	Table 4: <[DFL98] NNN> (Nos 1-551). Table 3: <[DFL98] Star NN> (Nos 1-39).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFL99]
[DFL99]	(Durret+Felenbok+Lobo+, 1999)
Write:	<<[DFL99] Star NNN>> <<[DFL99] Galaxy NNN>>
N:	101+466
Object:	* + G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table 3: N=101 stars misclassified as galaxies. Table 4: N=466 galaxies in the field of ACO 496. See also [SDG99b].
in source:	ACO 496
Ref:	=1999A&AS..139..525D
by	DURRET F. , FELENBOK P., LOBO C., SLEZAK E.
	Astron. Astrophys., Suppl. Ser., 139, 525-530 (1999)
	A catalogue of velocities in the direction of the cluster of galaxies Abell 496.
o	Table 3: <[DFL99] Star NNN> (Nos 1-101). Table 4: <[DFL99] Galaxy NNN> (Nos 1-466).
=E=	Catalogue in electronic form as J/A+AS/139/525
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFM2002]
[DFM2002]	(Deguchi+Fujii+Miyoshi+, 2002)
Write:	<<[DFM2002] NN>>
N:	15
Object:	SiO Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
in source:	NAME Gal Center
Ref:	=2002PASJ...54...61D
by	DEGUCHI S. , FUJII T., MIYOSHI M., NAKASHIMA J.
	Publ. Astron. Soc. Jap., 54, 61-70 (2002)
	Observations of SiO maser sources within a few parsec from the Galactic Center.
o	Table 2: <[DFM2002] NN> (Nos 1-15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFM2003]
[DFM2003]	(Damiani+Flaccomio+Micela+, 2003)
Write:	<<[DFM2003] NNN>>
N:	284
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of the open cluster NGC 2516.
in source:	NGC 2516
Ref:	=2003ApJ...588.1009D
by	DAMIANI F. , FLACCOMIO E., MICELA G., SCIORTINO S., HARNDEN F.R.Jr, MURRAY S.S., WOLK S.J., JEFFRIES R.D.
	Astrophys. J., 588, 1009-1024 (2003)
	Chandra X-ray observations of the young open cluster NGC 2516.
o	Table 4: <[DFM2003] NNN> (Nos 1-284). Table 4: <Cl* NGC 2516 JTH NNNNN> N=12 among (Nos 15496-15534) added.
=E=	Catalogue in electronic form as J/ApJ/588/1009
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFM2004]
[DFM2004]	(Damiani+Flaccomio+Micela+, 2004)
Write:	<<[DFM2004] NNN>>
N:	884
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra X-ray observations of the young cluster NGC 6530.
in source:	NGC 6530
Ref:	=2004ApJ...608..781D
by	DAMIANI F. , FLACCOMIO E., MICELA G., SCIORTINO S., HARNDEN F.R.Jr, MURRAY S.S.
	Astrophys. J., 608, 781-796 (2004)
	A deep Chandra X-ray observation of the rich young cluster NGC 6530. I. The X-ray source catalog and the cluster population.
o	Table 1: <[DFM2004] NNN> (Nos 1-884).
=E=	Catalogue in electronic form as J/ApJ/608/781
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFM2007]
[DFM2007]	(D'Elia+Fiore+Meurs+, 2007) (Not yet in Simbad)
Write:	<<[DFM2007] GRB 050730 abs N.NNN>>
N:	5
Object:	Absorber
Note:	VLT-UT2 UVES spectroscopy of GRB 050730.
Ref:	=2007A&A...467..629D
by	D'ELIA V. , FIORE F., MEURS E.J.A., CHINCARINI G., MELANDRI A., NORCI L., PELLIZZA L., PERNA R., PIRANOMONTE S., SBORDONE L., STELLA L., TAGLIAFERRI G., VERGANI S.D., WARD P., ANGELINI L., ANTONELLI L.A., BURROWS D.N., CAMPANA S., CAPALBI M., CIMATTI A., COSTA E., CUSUMANO G., DELLA VALLE M., FILLIATRE P., FONTANA A., FRONTERA F., FUGAZZA D., GEHRELS N., GIANNINI T., GIOMMI P., GOLDONI P., GUETTA D., ISRAEL G., LAZZATI D., MALESANI D., MARCONI G., MASON K., MEREGHETTI S., MIRABEL F., MOLINARI E., MORETTI A., NOUSEK J., PERRI M., PIRO L., STRATTA G., TESTA V., VIETRI M.
	Astron. Astrophys., 467, 629-639 (2007)
	UVES/VLT high resolution spectroscopy of GRB 050730 afterglow: probing the features of the GRB environment.
o	Text: <[DFM2007] GRB 050730 abs N.NNN> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFM2008]
[DFM2008]	(D'Elia+Fiore+Mathur+, 2008)
Write:	<<[DFM2008] NNN>>
N:	71
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS-I specroscopy of the 3C 295 cluster. Optical cross-identifications based on TNG DOLORES images. The sources were already cited but not designated in 2004A&A...422...11D. See also [DFM2008].
Ref:	=2008A&A...484..303D
by	D'ELIA V. , FIORE F., MATHUR S., COCCHIA F.
	Astron. Astrophys., 484, 303-309 (2008)
	The candidate filament close to the 3C295 galaxy cluster: optical and X-ray spectroscopy.
o	Paragraph 1. MRC 1138-206 is a probable misprint for MRC 1138-262.
o	Table 1: <[DFM2008] NNN> N=71 among (Nos 1-131).
=E=	Catalogue in electronic form as J/A+A/484/303
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFN2001]
[DFN2001]	(Doi+Furusawa+Nakata+, 2001)
Write:	<<[DFN2001] JHHMMSS.ss+DDMMSS.s>>
N:	8
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxies of SN 2001BC (see also [CAB2001]), and SN 2001CQ to 20001CW.
Ref:	=2001IAUC.7649....1D
by	DOI M. , FURUSAWA H., NAKATA F., OUCHI M., YASUDA N., MIYAZAKI S., KASHIKAWA N., KOMIYAMA Y., OHYAMA Y., YAGI M., AOKI K., HOOK I., PERLMUTTER S., ALDERING G.
	IAU Circ., 7649, 1-None (2001)
	Supernovae 2001cq, 2001cr, 2001cs, 2001ct, 2001cu, 2001cv, 2001cw.
o	<[DFN2001] JHHMMSS.ss+DDMMSS.s> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFO95]
[DFO95]	(Doi+Fukugita+Okamura+, 1995)= (Doi)
Write:	<<[DFO95] NNN>>
N:	450
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	Coma Cluster = ACO 1656
Ref:	=1995ApJS...97...77D
by	DOI M. , FUKUGITA M., OKAMURA S., TARUSAWA K.
	Astrophys. J., Suppl. Ser., 97, 77-88 (1995)
	Automated surface photometry for the Coma cluster galaxies: the catalog.
o	<[DFO95] NNN> N=450
=E=	Catalogue in electronic form as J/ApJS/97/77
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFP2006]
[DFP2006]	(Debattista+Ferreras+Pasquali+, 2006)
Write:	<<[DFP2006] VCC 128 PN>>
N:	2
Object:	Poss. G in Pair (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 images of VCC 128 reveal an apparently double nucleus.
in source:	VCC 128
Ref:	=2006ApJ...651L..97D
by	DEBATTISTA V.P. , FERRERAS I., PASQUALI A., SETH A., DE RIJCKE S., MORELLI L.
	Astrophys. J., 651L, 97-100 (2006)
	The binary nucleus in VCC 128: a candidate supermassive black hole in a dwarf elliptical galaxy.
o	Fig.1: <[DFP2006] VCC 128 PN> (Nos P1-P2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFP2009]
[DFP2009]	(D'Elia+Fiore+Perna+, 2009)
Write:	<<[DFP2009] GRB 080330 Host G>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Note:	VLT UVES observations of GRB 080330 and detection of the host galaxy.
Ref:	=2009A&A...503..437D
by	D'ELIA V. , FIORE F., PERNA R., KRONGOLD Y., VERGANI S.D., CAMPANA S., COVINO S., D'AVANZO P., FUGAZZA D., GOLDONI P., GUIDORZI C., MEURS E.J.A., NORCI L., PIRANOMONTE S., TAGLIAFERRI G., WARD P.
	Astron. Astrophys., 503, 437-444 (2009)
	UVES/VLT high resolution absorption spectroscopy of the GRB 080330 afterglow: a study of the GRB host galaxy and intervening absorbers.
o	<[DFP2009] GRB 080330 Host G> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFP2015]
[DFP2015]	(Di Cecco+Faustini+Paresce+, 2015)
Write:	<<[DFP2015] Her-NNN>>
N:	107
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Herschel PACS and SPIRE observations of N=107 far-IR point-like sources in the the cloud complex surrounding NGC 3603 YC.
in source:	NGC 3603
Ref:	=2015ApJ...799..100D
by	DI CECCO A. , FAUSTINI F., PARESCE F., CORRENTI M., CALZOLETTI L.
	Astrophys. J., 799, 100 (2015)
	Herschel Far-IR observations of the giant H II region NGC 3603.
o	Masers B-2, B-4, B-5 and B-6 (table 4 from 2010MNRAS.406.1487B) are not in SIMBAD.
o	Table 2: <[DFP2015] Her-NNN> (Nos 1-107).
=E=	Catalogue in electronic form as J/ApJ/799/100
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFP98]
[DFP98]	(De Ruiter+Fanti+Parma+, 1998)
Write:	<<[DFP98] B2 1637+29 AN>>
N:	7+5
Object:	G (SIMBAD class: Galaxy)
Note:	N=7 Galaxies (Nos A-G) in the field of the radio galaxy B2 1637+29, the galaxy 'A' has 3 components (Nos A1-A3), the galaxy 'C' has 2 components (Nos C1-C2). Optical image in Fig.1
Ref:	=1998A&A...337..711D
by	DE RUITER H.R. , FANTI R., PARMA P., LUB J., MORGANTI R., EKERS R.D.
	Astron. Astrophys., 337, 711-713 (1998)
	The peculiar radio galaxy B2 1637+29: a high velocity encounter of two galaxy groups?
o	Table 1: <[DFP98] B2 1637+29 AN> (Nos A-G), (Nos A1-A3), (Nos C1-C2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DFS
DFS	(Davis+Froebrich+Stanke+, 2009) (Not yet in Simbad)
*****	Avoid the usage of DFS, prefer [DFS2009]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 2dFS
2dFS	(2dF Spectroscopic survey)
Write:	<<2dFS NNNN>>
N:	4161
Object:	* (SIMBAD class: Star)
Note:	Catalogue of new spectral types for hot luminous stars in the SMC.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2004MNRAS.353..601E
by	EVANS C.J. , HOWARTH I.D., IRWIN M.J., BURNLEY A.W., HARRIES T.J.
	Mon. Not. R. Astron. Soc., 353, 601-623 (2004)
	A 2dF survey of the Small Magellanic Cloud.
o	Table 2: <2dFS NNNN> N=4161 among (Nos 1-5107).
=E=	Catalogue in electronic form as J/MNRAS/353/601
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DFS2009]
[DFS2009]	(Davis+Froebrich+Stanke+, 2009)= (DFS)
Write:	<<[DFS2009] NNN>> <<[DFS2009] IRS NNN>> <<[DFS2009] MMS NNN>>
N:	43+84+53
Object:	Outflow + (IR) + (mm) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	UKIRT WFCAM observations of N=43 new H2 outflows in Ori A (additions to [SMZ2002]). Spitzer IRAC and MIPS, and also IRAM 30m MAMBO observations of the likely outflow sources and dense cores that coincide with the source. These sources are numbered using the same calue given to the H2 outflow itself.
in source:	NAME Orion Ridge
Ref:	=2009A&A...496..153D
by	DAVIS C.J. , FROEBRICH D., STANKE T., MEGEATH S.T., KUMAR M.S.N., ADAMSON A., EISLOEFFEL J., GREDEL R., KHANZADYAN T., LUCAS P., SMITH M.D., VARRICATT W.P.
	Astron. Astrophys., 496, 153-176 (2009)
	A census of molecular hydrogen outflows and their sources along the Orion A molecular ridge. Characteristics and overall distribution.
o	Table 3: <[DFS2009] NNN> (Nos 101-143). Tables 2-3, col. "Outflow source": <[DFS2009] IRS NNN> N=54+30 among (Nos 1-76, 101-143). Tables 2-3, col. "1200um peak": <[DFS2009] MMS NNN> N=43+10 among (Nos 3-76, 103-131).
=E=	Catalogue in electronic form as <J/A+A/496/153/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DFV2017]
[DFV2017]	(Deshev+Finoguenov+Verdugo+, 2017)
Write:	<<[DFV2017] NNN>>
N:	407
Object:	G in ClG (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	MMT Hectospec spectroscopy of N=407 galaxies in the field of ACO 520 at z=0.2. See also [GBB2008].
in source:	ACO 520
Ref:	=2017A&A...607A.131D
by	DESHEV B. , FINOGUENOV A., VERDUGO M., ZIEGLER B., PARK C., HWANG H.S., HAINES C., KAMPHUIS P., TAMM A., EINASTO M., HWANG N., PARK B.-G.
	Astron. Astrophys., 607A, 131-131 (2017)
	Galaxy evolution in merging clusters: The passive core of the "Train Wreck" cluster of galaxies, A 520.
o	Table 1: <[DFV2017] NNN> (Nos 1-407).
=E=	Catalogue in electronic form as J/A+A/607/A131
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DG
DG	(Dorschner+Gurtler)
Write:	<<DG NNN>>
N:	192
Object:	RFN (SIMBAD class: RefNeb = Reflection Nebula)
Ref:	=1963AN....287..257D
by	DORSCHNER J. , GURTLER J.
	Astron. Nachr., 287, 257-260 (1963)
	Untersuchungen uber Reflexionsnebel am Palomar Sky Survey. I. Verzeichnis von Reflexionsnebeln.
o	<DG NNN> (Nos 1-192)
Origin	of the Acronym: L (1974Ap&SS..27....3M)
Details on Acronym: DG
DG	(Da Costa+Graham)
*****	Avoid the usage of DG, prefer [DG82]
Origin	of the Acronym: L (2004AJ....127.2674O)
Details on Acronym: DG
DG	(Dressler+Gunn)
*****	Avoid the usage of DG, prefer [DG92]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [DG2000]
[DG2000]	(Darling+Giovanelli, 2000)
Write:	<<[DG2000] HHMMm+DDMM>>
N:	12+24+19
Object:	OH Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	Survey of OH megamasers (OHM for the authors) in Arecibo: OH detections in the field of FSC IRAS galaxies.
Ref:	=2000AJ....119.3003D
by	DARLING J. , GIOVANELLI R.
	Astron. J., 119, 3003-3014 (2000)
	A search for OH megamasers at z>0.1. I. Preliminary results.
o	Table 3: <[DG2000] HHMMm+DDMM> N=12.
Ref:	=2001AJ....121.1278D
by	DARLING J. , GIOVANELLI R.
	Astron. J., 121, 1278-1293 (2001)
	A search for OH megamasers at z>0.1. II. Further results.
o	Table 3: <[DG2000] HHMMm+DDMM> N=24 added.
Ref:	=2002AJ....124..100D
by	DARLING J. , GIOVANELLI R.
	Astron. J., 124, 100-126 (2002)
	A search for OH megamasers at z>0.1. III. The complete survey.
o	Table 5: <[DG2000] HHMMm+DDMM> N=19 added.
=E=	Catalogue in electronic form as J/AJ/124/100
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DG2020]
[DG2020]	(Dekany+Grebel, 2020)
Write:	<<[DG2020] NNNNN>>
N:	13250
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Stat:	is completely incorporated in Simbad
Note:	N=13250 fundamental mode RR Lyrae (RRab) toward the Galactic Bulge. Use of VISTA Variables in the Via Lactea (VVV) Survey data. See also [DHG2018] and [DHG2019].
Ref:	=2020ApJ...898...46D
by	DEKANY I. , GREBEL E.K.
	Astrophys. J., 898, 46-46 (2020)
	Near-infrared search for fundamental-mode RR Lyrae stars toward the inner bulge by deep learning.
o	Table 3: <[DG2020] NNNNN> (Nos 1-13250).
=E=	Catalogue in electronic form as <J/ApJ/898/46/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [DG82]
[DG82]	(Da Costa+Graham, 1982)= (DG)
Write:	<<[DG82] N>>
N:	3
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Stat:	is completely incorporated in Simbad
Note:	CTIO observations. Observations of 3 globular cluster candidates in the field of NGC 55.
in source:	NGC 55
Ref:	=1982ApJ...261...70D
by	DA COSTA G.S. , GRAHAM J.A.
	Astrophys. J., 261, 70-76 (1982)
	Globular clusters in the Sculptor group galaxy NGC 55.
o	Table 1, Fig.1: <[DG82] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DG92]
[DG92]	(Dressler+Gunn, 1992)= (DG)
Write:	<<[DG92] N-NNN>>
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	1st ref., 1992ApJS...78....1D: Table 2: format '2-NNN', G in C 0949+4408. Table 3: format '3-NNN', G in C 0024+1654. N=19+2 are added later. Table 4: format '4-NNN', G in C 0939+4713 = GHO 093942+471306. N=96+5 are added later. Table 5: format '5-NNN', G in C 0303+1706 = GHO 030330+170630. N=24+2 are added later. Table 6: format '6-NNN', G in NAME 3C 295 Cluster. N=8 are added later. Table 7: format '7-NNN', G in C 1601+4253 = GHO 160134+425348. Table 8: format '8-NNN', G in C 0016+1609. N=13 are added later.
in source:	ClG 0949+4408
in source:	ClG 0024+1652 = HMS 0024+1654
in source:	ClG 0939+4713 = ACO 851
in source:	ClG 0303+1706
in source:	NAME 3C 295 Cluster
in source:	ClG 1601+4253
in source:	ClG 0016+1609 = 1E 0015.9+1609
Ref:	=1992ApJS...78....1D
by	DRESSLER A. , GUNN J.E.
	Astrophys. J., Suppl. Ser., 78, 1-60 (1992)
	Spectroscopy of galaxies in distant clusters. IV. A catalog of photometry and spectroscopy for galaxies in seven clusters with O.35<z< 0.55.
o	ClG 0909+4408, misprint for ClG 0949+4408
o	Table 2: <[DG92] 2-NNN> N=179 among 260. Table 3: <[DG92] 3-NNN> N=274 among 367. Table 4: <[DG92] 4-NNN> N=274 among 524. Table 5: <[DG92] 5-NNN> N=252 among 370. Table 6: <[DG92] 6-NNN> N≡200 among 241. Table 7: <[DG92] 7-NNN> N=307, Table 8-NNN> N=468 among 536.
Ref:	=1994ApJ...430..107D
by	DRESSLER A. , OEMLER A., BUTCHER H.R., GUNN J.E.
	Astrophys. J., 430, 107-120 (1994)
	The morphology of distant cluster galaxies. I. HST observations of CL 0939+4713.
o	Table: <[DG92] 4-NNN> N=96 added.
Ref:	=1997ApJS..110..213S
by	SMAIL I. , DRESSLER A., COUCH W.J., ELLIS R.S., OEMLER A., BUTCHER H., SHARPLES R.M.
	Astrophys. J., Suppl. Ser., 110, 213-226 (1997)
	A catalog of morphological types in 10 distant rich clusters of galaxies.
o	Table 1: CLG 1447+23 misprint for ClG 1447+26 (see coordinates)
o	Table 3: <[SDC97] a NNNN> N=8935. Table 3: <[DG92] 3-NNN> N=19 added, <[DG92] 5-NNN> N=24 added, <[DG92] 6-NNN> N=8 added, <[DG92] 8-NNN> N=13 added.
Ref:	=1999ApJS..122...51D
by	DRESSLER A. , SMAIL I., POGGIANTI B.M., BUTCHER H., COUCH W.J., ELLIS R.S., OEMLER A.Jr
	Astrophys. J., Suppl. Ser., 122, 51-80 (1999)
	A spectroscopic catalog of 10 distant rich clusters of galaxies.
o	The printed version gives a truncated format Cl HHMM. The complete format is ClG HHMM+DD in Simbad.
o	Tables 4a, 4b: <[DSP99] A 370 NNN>, <[DSP99] Cl HHMM+DD NNN>, <[DSP99] 3C 295 NNN>, N=424+253.
Ref:	=2000ApJ...541L..37F
by	FERRERAS I. , SILK J.
	Astrophys. J., 541, 37-40 (2000)
	How young are early-type cluster galaxies? Quantifying the young stellar component in a rich cluster at z=0.41.
o	T.1 : Galaxies 2016 and 833 not identified (not in [DG92] 4-...)
o	Table 4: <[DG92] 4-NNN> N=5 added.
=E=	Catalogue in electronic form as J/ApJS/78/1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DG95]
[DG95]	(Davidge+Grinder, 1995)
Write:	<<[DG95] EMSS HHMM a>> <<[DG95] ACO 2390 a>>
N:	3+1+3+2+1+1
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Table 2: in the format 'EMSS 0440' stands for 1E 0440+02.0, (Nos a-c) 'EMSS 0839' stands for 1E 0839+29.6, No. a 'EMSS 0906' stands for 1E 0906+11.1, (Nos a-c) 'EMSS 1231' stands for 1E 1231+15.7, (Nos a-b) 'EMSS 1455' stands for 1E 1455+22.6, No. a 'ACO 2390 a', No. a Maps in Fig. 1 to 6
in source:	1E 0440+02.0 = 1E 0440.5+0204 = ClG 0440+02
in source:	1E 0839+29.6 = 1E 0839.8+2938
in source:	1E 0906+11.1 = 1E 0906.5+1110
in source:	1E 1231+15.7 = 1E 1231.3+1542
in source:	1E 1455+22.6 = 1E 1455.0+2232 = ClG 1455+22
in source:	ACO 2390
Ref:	=1995AJ....109.1433D
by	DAVIDGE T.J. , GRINDER M.
	Astron. J., 109, 1433-1450 (1995)
	Stellar population gradients in bright cluster galaxies at z=0.2.
o	EMSS 0440+02 = 1E 0440+02.0, EMSS 0839+29 = 1E 0839+29.6, EMSS 0906+11 = 1E 00906+11.1, EMSS 1231+15 = 1E 1231+15.7, EMSS 1455+22 = 1E 1455+22.6
o	Table 2: <[DG95] EMSS 0440 a> N=3, <[DG95] EMSS 0839 a> N=1, <[DG95] EMSS 0906 a> N=3, <[DG95] EMSS 1231 a> N=2, <[DG95] EMSS 1455 a> N=1, <[DG95] ACO 2390 a> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DG97]
[DG97]	(Danziger+Gilmozzi, 1997)
Write:	<<[DG97] N-N>> <<[DG97] IPC N>>
N:	21+1
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Einstein X-ray deep survey In the format 'N-N', the first digit stands for the HRI exposures 1 to 4.
Ref:	=1997A&A...323...47D
by	DANZIGER I.J. , GILMOZZI R.
	Astron. Astrophys., 323, 47-55 (1997)
	The final optical identification content of the Einstein deep X-ray field in Pavo.
o	Table 1, col(1): [GMG83] NN
o	Table 1, col(2): <[DG97] N-N> N=21, <[DG97] IPC 1> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DG98]
[DG98]	(Dupin+Gry, 1998)
Write:	<<[DG98] Cloud A>>
N:	4
Object:	Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	HST HRS observations. Study of the line of sight towards the star 'bet CMa' to give a description of the ionized gas detected with Copernicus and discuss the nature of diffuse clouds embedded in the Local Bubble.
in source:	NAME Local Bubble
Ref:	=1998A&A...335..661D
by	DUPIN O. , GRY C.
	Astron. Astrophys., 335, 661-672 (1998)
	Diffuse ionized gas toward β Canis Majoris.
o	<[DG98] Cloud A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DGA2006]
[DGA2006]	(DeLaney+Gaensler+Arons+, 2006)
Write:	<<[DGA2006] JHHMMSS+DDMMSS>> <<[DGA2006] arc a>>
N:	4+2
Object:	(X) + arc (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	New and archival Chandra and ROSAT data of the X-ray emission around PSR 1509-58.
Ref:	=2006ApJ...640..929D
by	DELANEY T. , GAENSLER B.M., ARONS J., PIVOVAROFF M.J.
	Astrophys. J., 640, 929-940 (2006)
	Time variability in the X-ray nebula powered by pulsar B1509-58.
o	Paragr. 2: <[DGA2006] JHHMMSS+DDMMSS> N=4. Fig.1: <[DGA2006] arc a> (Nos a-b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DGA2015]
[DGA2015]	(D'Orazi+Gratton+Angelou+, 2015)
Write:	<<[DGA2015] NGC 1904 NNNNN>> <<[DGA2015] NGC 2808 NNNNN>> <<[DGA2015] NGC 362 NNNNN>>
N:	48+69+68
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT FLAMES spectroscopic observations of N=48+69+68 RGB stars in three globular cluster giants: NGC 1904, NGC 2808, and NGC 362.
in source:	NGC 1904
in source:	NGC 2808
in source:	NGC 362
Ref:	=2015MNRAS.449.4038D
by	D'ORAZI V. , GRATTON R.G., ANGELOU G.C., BRAGAGLIA A., CARRETTA E., LATTANZIO J.C., LUCATELLO S., MOMANY Y., SOLLIMA A., BECCARI G.
	Mon. Not. R. Astron. Soc., 449, 4038-4047 (2015)
	Lithium abundances in globular cluster giants: NGC 1904, NGC 2808, and NGC 362.
o	Table 1: <[DGA2015] NGC 1904 NNNNN> N=48 among (Nos 622-12004), <[DGA2015] NGC 2808 NNNNN> N=69 among (Nos 7431-63132), <[DGA2015] NGC 362 NNNNN> N=68 among (Nos 1155-19167).
=E=	Catalogue in electronic form as J/MNRAS/449/4038
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DGB2001]
[DGB2001]	(Dupac+Giard+Bernard+, 2001)
Write:	<<[DGB2001] Cloud N>>
N:	4
Object:	Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	PRONAOS observations.
in source:	Ori A = M 42
Ref:	=2001ApJ...553..604D
by	DUPAC X. , GIARD M., BERNARD J.-P., LAMARRE J.-M., MENY C., PAJOT F., RISTORCELLI I., SERRA G., TORRE J.-P.
	Astrophys. J., 553, 604-612 (2001)
	Submillimeter mapping and analysis of cold dust condensations in the Orion M42 star-forming complex.
o	Fig.2, Table 2: <[DGB2001] Cloud N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DGB2002]
[DGB2002]	(Dupac+Giard+Bernard+, 2002)
Write:	<<[DGB2002] Cloud A>>
N:	4
Object:	(submm) Cloud (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	PRONAOS observations. N=4 submillimeter condensations in M 17.
in source:	M 17 = NGC 6618
Ref:	=2002A&A...392..691D
by	DUPAC X. , GIARD M., BERNARD J.-P., BOUDET N., LAMARRE J.-M., MENY C., PAJOT F., POINTECOUTEAU E., RISTORCELLI I., SERRA G., STEPNIK B., TORRE J.-P.
	Astron. Astrophys., 392, 691-698 (2002)
	Submillimeter dust emission of the M 17 complex measured with PRONAOS.
o	Table 1: <[DGB2002] Cloud A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DGB2017]
[DGB2017]	(Dabhade+Gaikwad+Bagchi+, 2017)
Write:	<<[DGB2017] GRGNN>>
N:	25
Object:	Giant Radio G (SIMBAD class: RadioG = Radio Galaxy)
Note:	Identification of N=25 Giant Radio Galaxies (GRGs). Use of archival NVSS images, SDSS data and VLA FIRST survey.
Ref:	=2017MNRAS.469.2886D
by	DABHADE P. , GAIKWAD M., BAGCHI J., PANDEY-POMMIER M., SANKHYAYAN S., RAYCHAUDHURY S.
	Mon. Not. R. Astron. Soc., 469, 2886-2906 (2017)
	Discovery of giant radio galaxies from NVSS: radio and infrared properties.
o	Table 1: <[DGB2017] GRGNN> (Nos 1-25).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DGC
DGC	(Drake, Galaxy Cluster)
*****	Avoid the usage of DGC, prefer [D2005c]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DGC92]
[DGC92]	(Dubner+Giacani+Cappa de Nicolau+, 1992)= (GS)
Write:	<<[DGC92] LLL+B+VVV>> <<[DGC92] LLL.l+B+VVV>> <<[DGC92] LLL.l+B.b+VVV>>
N:	8
Object:	HI Shell (SIMBAD class: HIshell = Interstellar Shell)
Stat:	is completely incorporated in Simbad
Note:	Page 513: N=8 new Galactic Shells
Ref:	=1992A&AS...96..505D
by	DUBNER G. , GIACANI E., CAPPA DE NICOLAU C., REYNOSO E.
	Astron. Astrophys., Suppl. Ser., 96, 505-523 (1992)
	A study of the neutral hydrogen in direction to the Gum nebula.
o	Page 513: <[DGC92] LLL+B+VVV>, <[DGC92] LLL.l+B+VVV>, <[DGC92] LLL.l+B.b+VVV>, N=8.
Details on Acronym: DGF
DGF	(Debes+Ge+Ftaclas)
Write:	<<DGF N>> <<DGF WD HHMM+DDd CN>>
N:	7+4
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	CFHT observations of WDs: 7 new extragalactic objects are found in the fields of view. 2 WD have candidate companions.
Ref:	=2006AJ....131..640D
by	DEBES J.H. , GE J., FTACLAS C.
	Astron. J., 131, 640-647 (2006)
	Cool customers in the stellar graveyard. III. Limits to substellar objects around nearby white dwarfs using the Canada-France-Hawaii telescope.
o	Table 3: <DGF N> (Nos 1-7). Fig.2: <DGF WD 2341+321 CN> (Nos C1-C2). Fig.5 <DGF WD 0208+395 CN> (Nos C1-C2).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DGG2000]
[DGG2000]	(Donato+Garzia+Gonano+, 2000)
Write:	<<[DGG2000] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Stat:	is completely incorporated in Simbad
Note:	Discovery of a new nova in M 31.
in source:	M 31 = NGC 224
Ref:	=2000IAUC.7516R...1D
by	DONATO L. , GARZIA S., GONANO V., SOSTERO G., KORLEVIC K.
	IAU Circ., 7516, 1-None (2000)
	Nova in M 31.
o	<[DGG2000] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DGG95]
[DGG95]	(Duric+Gordon+Goss+, 1995)
Write:	<<[DGG95] NN>>
N:	53
Object:	SNR (SIMBAD class: SNRemnant = SuperNova Remnant)
Stat:	is completely incorporated in Simbad
Note:	Radio continuum observations of SNRs in M 33.
in source:	M 33 = NGC 598
Ref:	=1995ApJ...445..173D
by	DURIC N. , GORDON S.M., GOSS W.M., VIALLEFOND F., LACEY C.
	Astrophys. J., 445, 173-181 (1995)
	The relativistic ISM in M 33: the role of the supernova remnants.
o	Table 1, col(2): SNR format not used in SIMBAD.
o	Table 1: <[DGG95] NN> (Nos 1-53)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DGH2001]
[DGH2001]	(Drinkwater+Gregg+Holman+, 2001)
Write:	<<[DGH2001] JHHMMSS.ss+DDMMSS.s>> <<[DGH2001] Name N>>
N:	3+7
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Observations of the Fornax Cluster. The sample included 10 objects not in the FCC: N=3 in Table 3, with spectra dominated by light from a foreground galactic star. N=7 background galaxies 'Name 1' to 'Name 7' in Appendix A1 and A2, with cross-id in Table 7.
Ref:	=2001MNRAS.326.1076D
by	DRINKWATER M.J. , GREGG M.D., HOLMAN B.A., BROWN M.J.I.
	Mon. Not. R. Astron. Soc., 326, 1076-1094 (2001)
	The evolution and star formation of dwarf galaxies in the Fornax Cluster.
o	Table 3: <[DGH2001] JHHMMSS.ss+DDMMSS.s> N=3. Tables A1, A2: <[DGH2001] Name N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DGH2003]
[DGH2003]	(Dahlen+GOODS TREASURY Team+HUBBLE Higher-z supernova Team, 2003)
Write:	<<[DGH2003] JHHMMSS.ss+DDMMSS.s>>
N:	6
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations. Host galaxies of SN 2003AZ, SN 2003BA, SN 2003BB, SN 2003BC, SN 2003BD, SN 2003BE.
Ref:	=2003IAUC.8081....1D
by	DAHLEN T. , (The GOODS Treasury Team), (The Hubble Higher-Z Supernova Team)
	IAU Circ., 8081, 1-None (2003)
	Supernovae 2003az, 2003ba, 2003bb, 2003bc, 2003bd, 2003be.
o	<[DGH2003] JHHMMSS.ss+DDMMSS.s> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DGH2004]
[DGH2004]	(Darling+Giovanelli+Haynes+, 2004)
Write:	<<[DGH2004] QSO J2354+4553 abs N.NN>>
N:	1
Object:	DLA
Note:	First detection of GBT DLA survey toward the QSO J2354+4553 = 4C +45.51.
Ref:	=2004ApJ...613L.101D
by	DARLING J. , GIOVANELLI R., HAYNES M.P., BOLATTO A.D., BOWER G.C.
	Astrophys. J., 613, 101-104 (2004)
	Detection of 21 centimeter H I absorption at z=0.78 in a survey of radio continuum sources.
o	<[DGH2004] QSO J2354+4553 abs 0.78> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DGH2009]
[DGH2009]	(Da Rio+Gouliermis+Henning, 2009)
Write:	<<[DGH2009] NN>> <<[DGH2009] A>>
N:	15+3
Object:	* + subclusters (SIMBAD class: Star)
Note:	HST/ACS photometry of the stellar association LH 95.
in source:	LH 95
Ref:	=2009ApJ...696..528D
by	DA RIO N. , GOULIERMIS D.A., HENNING T.
	Astrophys. J., 696, 528-545 (2009)
	The complete initial mass function down to the subsolar regime in the Large Magellanic Cloud with Hubble space telescope ACS observations.
o	Table 1: <[DGH2009] NN> (Nos 1-15). Table 2, Fig. 4: <[DGH2009] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DGI91]
[DGI91]	(Demers+Grondin+Irwin+, 1991)= (DGIK)
Write:	<<[DGI91] NNN>>
N:	196 among 986
Object:	* in Assoc. (SIMBAD class: Star)
in source:	Magellanic Clouds:Magellanic Bridge = Magellanic Bridge
in source:	IDK 6
Ref:	=1991AJ....101..911D
by	DEMERS S. , GRONDIN L., IRWIN M.J., KUNKEL W.E.
	Astron. J., 101, 911-921 (1991)
	Young stars between the Magellanic clouds. II. An association on the Far-West side of the LMC halo.
o	<[DGI91] NNN> N=196 among (Nos 8-986).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DGI99]
[DGI99]	(Dey+Graham+Ivison+, 1999)= (ERO)
Write:	<<[DGI99] JHHMMSS+DDMM.m>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=2 Extremely Red Objects.
Ref:	=1999ApJ...519..610D
by	DEY A. , GRAHAM J.R., IVISON R.J., SMAIL I., WRIGHT G.S., LIU M.C.
	Astrophys. J., 519, 610-621 (1999)
	Observations of a z = 1.44 dusty, ultraluminous galaxy and implications for deep submillimeter surveys.
o	<[DGI99] JHHMMSS+DDMM.m> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DGIK
DGIK	(Demers+Grondin+Irwin+Kunkel)
*****	Avoid the usage of DGIK, prefer [DGI91]
Origin	of the Acronym: L (2005A&A...429.1025L)
Details on Acronym: [DGK2000]
[DGK2000]	(Douglas+Gerssen+Kuijken+, 2000)
Write:	<<[DGK2000] JHHMMSS.ss+DDMMSS.s>>
N:	53+14
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Search for PN in M 94: N=53 in the major-axis field and N=14 in the minor-axis field.
in source:	M 94
Ref:	=2000MNRAS.316..795D
by	DOUGLAS N.G. , GERSSEN J., KUIJKEN K., MERRIFIELD M.R.
	Mon. Not. R. Astron. Soc., 316, 795-802 (2000)
	Using slitless spectroscopy to study the kinematics of the planetary nebula population in M94.
o	(Erratum) erratum vol.328, p.1200 (2001)
o	Tables 2, 3: <[DGK2000] JHHMMSS.ss+DDMMSS.s> N=53+14.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DGK2015]
[DGK2015]	(Dai+Griffin+Kochanek+, 2015)= (SACS) = (SWCL)
Write:	<<[DGK2015] SACS JHHMMSS.s+DDMMSS>> <<[DGK2015] SWCL JHHMMSS.s+DDMMSS>>
N:	22563+442
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Catalog of N=22563 point sources and N=442 extended sources, as part of the Swift AGN and Cluster Survey (SACS). Use of archival Swift XRT observations of GRB fields.
Ref:	=2015ApJS..218....8D
by	DAI X. , GRIFFIN R.D., KOCHANEK C.S., NUGENT J.M., BREGMAN J.N.
	Astrophys. J., Suppl. Ser., 218, 8 (2015)
	The Swift AGN and Cluster Survey. I. Number counts of AGNs and galaxy clusters.
o	Tables 1, 2, 3: <[DGK2015] SACS JHHMMSS.s+DDMMSS> N=22563. Table 4: <[DGK2015] SWCL JHHMMSS.s+DDMMSS> N=442.
=E=	Catalogue in electronic form as J/ApJS/218/8
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DGL
DGL	(De Luca+Giannini+Lorenzetti+)
Write:	<<DGL NN>>
N:	13
Object:	(smm) (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	NTT SofI and ESO 3.6m telescope Timmi2 observations at La Sillai of the Vela D molecular cloud.
in source:	VMR D
Ref:	=2007A&A...474..863D
by	DE LUCA M. , GIANNINI T., LORENZETTI D., MASSI F., ELIA D., NISINI B.
	Astron. Astrophys., 474, 863-872 (2007)
	Near- and far-infrared counterparts of millimeter dust cores in the Vela molecular ridge cloud D.
o	Table 1 : 2MASS source 2M 16489 not identified. Misprint in δ ? (-43 31 53.63 instead of -43 13 53.63)
o	Table 1, col(id, Timmi2): <DGL NN> (Nos 1-13).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DGM2002]
[DGM2002]	(Dobrzycki+Groot+Macri+, 2002)
Write:	<<[DGM2002] JHHMMSS.ss+DDMMSS.s>>
N:	4
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	Discovery of 4 QSOs located behind the LMC, identified via spectroscopy of optical counterparts to X-ray sources found seredipitously by the CXO satellite. All 4 QSOs have archival photometry from the OGLE-II.
Ref:	=2002ApJ...569L..15D
by	DOBRZYCKI A. , GROOT P.J., MACRI L.M., STANEK K.Z.
	Astrophys. J., 569, 15-18 (2002)
	Discovery of four X-ray quasars behind the Large Magellanic Cloud.
o	Table 1: <[DGM2002] JHHMMSS.ss+DDMMSS.s> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DGP2006]
[DGP2006]	(De Pasquale+Grupe+Poole+, 2006)
Write:	<<[DGP2006] JHHMMSS.s+DDMMSS.s>>
N:	1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Swift observatory observations of the field of GRB 050712. An unknown X-ray source is found.
Ref:	=2006MNRAS.370.1859D
by	DE PASQUALE M. , GRUPE D., POOLE T.S., BREEVELD A.A., ZANE S., ROSEN S.R., PAGE M.J., MASON K.O., BURROWS D.N., KRIMM H.A., GEHRELS N., NOUSEK J.A., ROMING P.W.A., KOBAYASHI S., ZHANG B.
	Mon. Not. R. Astron. Soc., 370, 1859-1866 (2006)
	Swift observations of GRB 050712.
o	In Intro. : GRB 030309 not identified, could be a misprint.
o	Text: <[DGP2006] JHHMMSS.s+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DGP2020]
[DGP2020]	(D'Amato+Gilli+Prandoni+, 2020)
Write:	<<[DGP2020] aN>>
N:	4
Object:	G (SIMBAD class: Galaxy)
Note:	ALMA Band 3 observations of N=4 galaxies in the field of QSO J1030+0524. See also [GMP2019].
Ref:	=2020A&A...641L...6D
by	D'AMATO Q. , GILLI R., PRANDONI I., VIGNALI C., MASSARDI M., MIGNOLI M., CUCCIATI O., MORISHITA T., DECARLI R., BRUSA M., CALURA F., BALMAVERDE B., CHIABERGE M., LIUZZO E., NANNI R., PECA A., PENSABENE A., TOZZI P., NORMAN C.
	Astron. Astrophys., 641L, 6-6 (2020)
	Discovery of molecular gas fueling galaxy growth in a protocluster at z = 1.7.
o	Fig. 1, Table 1: <[DGP2020] aN> (Nos a0-a3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DGPS
DGPS	(Swift Deep Galactic Plane Survey) (Not yet in Simbad)
Write:	<<DGPS JHHMMSS.s+DDMMSS>>
N:	802+126
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	The Swift Deep Galactic Plane Survey (DGPS) is a Swift Key Project consisting of 380 tiled pointings covering ∼40 sq. deg of the Galactic plane between longitude 10°<\|l\|<30° and latitude \|b\|<0.5°. The main survey goal is to produce a rich sample of new X-ray sources and transients. Catalog of N=928 sources detected during Phase I observations. Use of the Living Swift-XRT Point-source catalog (LSXPS).
Ref:	=2023ApJS..269...49O
by	O'CONNOR B. , KOUVELIOTOU C., EVANS P.A., GORGONE N., VAN KOOTEN A.J., GAGNON S., YANG H., BARING M.G., BELLM E., BENIAMINI P., BRINK J., BUCKLEY D.A.H., CENKO S.B., EGBO O.D., GOGUS E., GRANOT J., HAILEY C., HARE J., HARRISON F., HARTMANN D., VAN DER HORST A.J., HUPPENKOTHEN D., KAPER L., KARGALTSEV O., KENNEA J.A., MUKAI K., SLANE P.O., STERN D., TROJA E., WADIASINGH Z., WIJERS R.A.M.J., WOUDT P., YOUNES G.
	Astrophys. J., Suppl. Ser., 269, 49 (2023)
	The Swift Deep Galactic Plane Survey (DGPS) Phase I Catalog.
o	Tables 2-3: <DGPS JHHMMSS.s+DDMMSS> N=802+126.
=E=	Catalogue in electronic form as <J/ApJS/269/49/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DGR2004]
[DGR2004]	(Dubner+Giacani+Reynoso+, 2004)
Write:	<<[DGR2004] Cloud A>>
N:	2
Object:	Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	SEST CO observations. [DGR99] Cloud 3 in SNR 18.8+0.3 is resolved in two components designated as Cloud A and B.
in source:	SNR G018.8+00.3
Ref:	=2004A&A...426..201D
by	DUBNER G. , GIACANI E., REYNOSO E., PARON S.
	Astron. Astrophys., 426, 201-212 (2004)
	The molecular clouds in the environs of the supernova remnants G349.7+0.2 and G18.8+0.3.
o	Table 3: <[DGR2004] Cloud A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DGR99]
[DGR99]	(Dubner+Giacani+Reynoso+, 1999)
Write:	<<[DGR99] Cloud N>> <<[DGR99] Feature A>>
N:	5+1
Object:	Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	Molecular clouds adjacent to SNR 18.8+0.3 observed in HI, CO, and OH. See also [DGR2004].
in source:	SNR G018.8+00.3
Ref:	=1999AJ....118..930D
by	DUBNER G. , GIACANI E., REYNOSO E., GOSS W.M., ROTH M., GREEN A.
	Astron. J., 118, 930-941 (1999)
	Interaction of the supernova remnant G18.8+0.3 with the surrounding medium.
o	Table 1: <[DGR99] Cloud N> (Nos 1-5), <[DGR99] Feature A> (No. A).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DGS
DGS	(Dressler+Gunn+Schneider)
*****	Avoid the usage of DGS, prefer SDG
Origin	of the Acronym: L (1985ApJ...294...70D)
Details on Acronym: [DGS2003]
[DGS2003]	(Donato+Gliozzi+Sambruna+, 2003)
Write:	<<[DGS2003] PKS HHMM+DDd A>> <<[DGS2003] 3C 371 A>> <<[DGS2003] BL Lac A>> <<[DGS2003] 1ES HHMM+DDd A>>
N:	7+7+7+10+11+7
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of the X-ray environment of 6 Bl Lac objects.
Ref:	=2003A&A...407..503D
by	DONATO D. , GLIOZZI M., SAMBRUNA R.M., PESCE J.E.
	Astron. Astrophys., 407, 503-513 (2003)
	Chandra observations of the X-ray environment of BL Lacs.
o	Table 5: <[DGS2003] PKS 0548-322 A> (Nos A-G), <[DGS2003] 3C 371 A> (Nos A-G), <[DGS2003] PKS 2005-489 A> (Nos A-G), <[DGS2003] BL Lac A> (Nos A-L, J, K missing), <[DGS2003] 1ES 2321+514 A> (Nos A-M, J, K missing), <[DGS2003] 1ES 2344+514 A> (Nos A-G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DGS2006]
[DGS2006]	(De Gregorio-Monsalvo+Gomez+Suarez+, 2006) (Not yet in Simbad)
Write:	<<[DGS2006] CB 3 A>>
N:	5
Object:	H2O Maser (SIMBAD class: Maser)
Note:	VLA observations of [CB88] 3.
in source:	[CB88] 3
Ref:	=2006AJ....132.2584D
by	DE GREGORIO-MONSALVO I. , GOMEZ J.F., SUAREZ O., KUIPER T.B.H., ANGLADA G., PATEL N.A., TORRELLES J.M.
	Astron. J., 132, 2584-2595 (2006)
	High-resolution observations of water masers in Bok globules.
o	Table 1: phase calibrator J0136+478 is not identified.
o	Table 2: <[DGS2006] CB 3 A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DGS2013]
[DGS2013]	(Dahle+Gladders+Sharon+, 2013)
Write:	<<[DGS2013] SDSS J2222+2745>> <<[DGS2013] SDSS J2222+2745 lens>> <<[DGS2013] SDSS J2222+2745A>> <<[DGS2013] SDSS J2222+2745 GN>> <<[DGS2013] SDSS J2222+2745 arc>> <<[DGS2013] WD>>
N:	1+1+6+3+1+1
Object:	Grav. lens system + Grav. lens + Grav. lensed image of a QSO + G + WD* (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	NOT ALFOSC observations of N=1 gravitational lens system producing six images of a quasar lensed by a foreground galaxy cluster. Use of SDSS data.
Ref:	=2013ApJ...773..146D
by	DAHLE H. , GLADDERS M.D., SHARON K., BAYLISS M.B., WUYTS E., ABRAMSON L.E., KOESTER B.P., GROENEBOOM N., BRINCKMANN T.E., KRISTENSEN M.T., LINDHOLMER M.O., NIELSEN A., KROGAGER J.-K., FYNBO J.P.U.
	Astrophys. J., 773, 146 (2013)
	SDSS J2222+2745: a gravitationally lensed sextuple quasar with a maximum image separation of 15.''1 discovered in the Sloan giant arcs survey.
o	<[DGS2013] SDSS J2222+2745> N=1, <[DGS2013] SDSS J2222+2745 lens> N=1, <[DGS2013] SDSS J2222+2745A> (Nos A-F), <[DGS2013] SDSS J2222+2745 GN> (Nos G1-G3), <[DGS2013] SDSS J2222+2745 arc> N=1, <[DGS2013] WD> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DGSW
DGSW	(Downes+Goss+Schwarz+Wouterloot)
Write:	<<DGSW NN>>
N:	74
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1979A&AS...35....1D
by	DOWNES D. , GOSS W.M., SCHWARZ U.J., WOUTERLOOT J.G.A.
	Astron. Astrophys., Suppl. Ser., 35, 1-22 (1979)
	Compact radio sources in the Galactic Center region.
o	<DGSW NN> (Nos 1-74)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [DGT2000]
[DGT2000]	(Dieball+Grebel+Theis, 2000)
Write:	<<[DGT2000] NN>>
N:	22
Object:	* in Cl* (SIMBAD class: Star)
Note:	* in the clusters [SL63] 353 and 349, or in the field of the clusters, or foreground stars. Chart in Fig.1.
in source:	[SL63] 353
in source:	[SL63] 349
Ref:	=2000A&A...358..144D
by	DIEBALL A. , GREBEL E.K., THEIS C.
	Astron. Astrophys., 358, 144-153 (2000)
	Studies of binary star cluster candidates in the bar of the LMC. I. SL 353 and SL 349.
o	Table 5: <[DGT2000] NN> (Nos 1-22).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DGT2001]
[DGT2001]	(Donato+Ghisellini+Tagliaferri+, 2001)
Write:	<<[DGT2001] BHHMM+DDd>> <<[DGT2001] BHHMM+DDMM>> <<[DGT2001] JHHMM+DDd>> <<[DGT2001] JHHMM+DDMM>>
N:	268
Object:	Blazar (SIMBAD class: Blazar)
Stat:	is completely incorporated in Simbad
Note:	N=268 blazars detected in the X-ray band from the data of the 5 satellites Einstein, EXOSAT, ROSAT, ASCA, and BeppoSAX. The authors used a format without B (1950 coordinates) or J (2000 coordinates), and there are N=60 objects with 2000 coordinates 'JHHMM+DDd' or 'JHHMM+DDMM' in SIMBAD, and N=208 objects with 1950 coordinates 'BHHMM+DDd' or 'BHHMM+DDMM' in SIMBAD.
Ref:	=2001A&A...375..739D
by	DONATO D. , GHISELLINI G., TAGLIAFERRI G., FOSSATI G.
	Astron. Astrophys., 375, 739-751 (2001)
	Hard X-ray properties of blazars.
o	Table 5: Authors used a designation 'HHMM+DDd' or 'HHMM+DDMM' without specification which ones are B (1950 coordinates) and which ones are J (2000 coordinates). In SIMBAD and in the CDS catalogue, this is specified.
o	Table 5: <[DGT2001] BHHMM+DDd> or <[DGT2001] BHHMM+DDMM> N=208, <[DGT2001] JHHMM+DDd> or <[DGT2001] JHHMM+DDMM> N=60.
=E=	Catalogue in electronic form as J/A+A/375/739
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DGVW
DGVW	(Davis+Gelato-Volders+Westerhout)
*****	Avoid the usage of DGVW, prefer [DGW65]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [DGW65]
[DGW65]	(Davis+Gelato-Volders+Westerhout, 1965)= (D) = (DGVW)
Write:	<<[DGW65] NNN>>
N:	149
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Ref:	=1965BAN....18...42D
by	DAVIS M.M. , GELATO-VOLDERS L., WESTERHOUT G.
	Bull. Astron. Inst. Netherlands, 18, 42-50 (1965)
	A catalogue of discrete sources observed at 400 Mc/s.
o	<[DGW65] NNN> (Nos 1-149)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DH2015]
[DH2015]	(Dahm+Hillenbrand, 2015)
Write:	<<[DH2015] NN>> <<[DH2015] JHHMMSS.ss+DDMMSS.s>>
N:	72+2435
Object:	* + (Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	KPNO 0.9m telescope T2KA CCD imaging survey of N=72+2435 sources in NGC 7129.
in source:	NGC 7129
Ref:	=2015AJ....149..200D
by	DAHM S.E. , HILLENBRAND L.A.
	Astron. J., 149, 200 (2015)
	An optical survey of the partially embedded young cluster in NGC 7129.
o	Table 1: <IfAHA NNN> (Nos 763-821) added. Table 3: <[DH2015] NN> (Nos 1-72). Table 4: <[DH2015] JHHMMSS.ss+DDMMSS.s> N=2435.
o	S3-U1350 is a probable misprint for S2-U1350.
=E=	Catalogue in electronic form as J/AJ/149/200
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DH96]
[DH96]	(Dachs+Hummel, 1996)
Write:	<<[DH96] NN>>
N:	64
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT PSPC observations
in source:	NGC 2516
Ref:	=1996A&A...312..818D
by	DACHS J. , HUMMEL W.
	Astron. Astrophys., 312, 818-832 (1996)
	ROSAT survey of stellar X-ray sources in the young open cluster NGC 2516.
o	Table 2, col.(2), Table 4, col(3): designations not in SIMBAD. Table 3: DK = Cl* NGC 2516 DAC
o	Table 2: <[DH96] NN> (Nos 1-64)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DH98]
[DH98]	(Dolphin+Hunter, 1998)
Write:	<<[DH98] LH 77 xxxx.xxx+yyyy.yyy>> <<[DH98] NGC NNNN xxxx.xxx+yyyy.yyy>> <<[DH98] SL 502 xxxx.xxx+yyyy.yyy>> <<[DH98] BWW xxxx.xxx+yyyy.yyy>>
N:	149140
Object:	* (SIMBAD class: Star)
Note:	UBV photometry in 7 fields within the Shapley Constellation III. Background Fields 'BNW' and 'BSE' are not objects.
in source:	Shapley III
Ref:	=1998AJ....116.1275D
by	DOLPHIN A.E. , HUNTER D.A.
	Astron. J., 116, 1275-1285 (1998)
	Recent star formation in Shapley constellation III in the Large Magellanic Cloud.
o	Tables 2: <[DH98] LH 77 xxxx.xxx+yyyy.yyy>, <[DH98] NGC NNNN xxxx.xxx+yyyy.yyy>, <[DH98] SL 502 xxxx.xxx+yyyy.yyy>, <[DH98] BWW xxxx.xxx+yyyy.yyy>, N=149140.
=E=	Catalogue in electronic form as J/AJ/116/1275
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DHB2007]
[DHB2007]	(Dow-Hygelund+Holden+Bouwens+, 2007)
Write:	<<[DHB2007] BD NN>> <<[DHB2007] UDF PFs1 iN>> <<[DHB2007] UDF PFs iN>> <<[DHB2007] GOODS i6 0>>
N:	14+2+5+1
Object:	G (SIMBAD class: Galaxy)
Note:	Keck I LRIS and VLT FORS2 observations of Lyman-alpha galaxies in two fields: RDCS J1252-2927 and UDF Parallel Spectroscopic Field.
Ref:	=2007ApJ...660...47D
by	DOW-HYGELUND C.C. , HOLDEN B.P., BOUWENS R.J., ILLINGWORTH G.D., VAN DER WEL A., FRANX M., VAN DOKKUM P.G., FORD H., ROSATI P., MAGEE D., ZIRM A.
	Astrophys. J., 660, 47-61 (2007)
	Spectroscopy of z ~ 6 i-dropout galaxies: frequency of Lyα emission and the sizes of Lyα-emitting galaxies.
o	Fig.10, Tables 1, 3: <[DHB2007] BD NN> N=14 among (Nos 00-66). Fig.10, Tables 2, 4: <[DHB2007] UDF PFs1 iN> (Nos i0, i1, i9), <[DHB2007] UDF PFs iN> N=5 among (Nos i0-i9), <[DHB2007] GOODS i6 0> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DHB2009]
[DHB2009]	(Daemgen+Hormuth+Brandner+, 2009)
Write:	<<[DHB2009] WASP-2/C>> <<[DHB2009] TrES-N/C>>
N:	1+2
Object:	* (SIMBAD class: Star)
Note:	Observations with the AstraLux camera at the 2.2m Calar Alto telescope.
Ref:	=2009A&A...498..567D
by	DAEMGEN S. , HORMUTH F., BRANDNER W., BERGFORS C., JANSON M., HIPPLER S., HENNING T.
	Astron. Astrophys., 498, 567-574 (2009)
	Binarity of transit host stars. Implications for planetary parameters.
o	Table 4: <[DHB2009] WASP-2/C> N=1, <[DHB2009] TrES-N/C> (Nos TrES-2/C, TrES-4/C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DHC2002]
[DHC2002]	(Dawson+Holzapfel+Carlstrom+, 2002) (Not yet in Simbad)
Write:	<<[DHC2002] +xxx.x+yyy.y>>
N:	38
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	N=38 radio point-sources from the VLA in BDF fields (BIMA Deep Field). See also [HCG2000].
Ref:	=2002ApJ...581...86D
by	DAWSON K.S. , HOLZAPFEL W.L., CARLSTROM J.E., JOY M., LAROQUE S.J., MILLER A.D., NAGAI D.
	Astrophys. J., 581, 86-95 (2002)
	Measurement of arcminute-scale cosmic microwave background anisotropy with the Berkeley-Illinois-Maryland association array.
o	Table 2:<[DHC2002] +xxx.x+yyy.y> N=38.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DHC2006]
[DHC2006]	(Dawson+Holzapfel+Carlstrom+, 2006)
Write:	<<[DHC2006] BDFNN +xxx.x+yyy.y>> <<[DHC2006] HDF +xxx.x+yyy.y>>
N:	26+28+6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA 4.8GHz, 8GHz, and 30GHz observations of the BIMA Deep Fields (BDF) and the HDF.
Ref:	=2006ApJ...647...13D
by	DAWSON K.S. , HOLZAPFEL W.L., CARLSTROM J.E., JOY M., LAROQUE S.J.
	Astrophys. J., 647, 13-24 (2006)
	Final results from the BIMA CMB anisotropy survey and search for a signature of the Sunyaev-Zel'dovich effect.
o	Tables 2, 3: <[DHC2006] BDFNN +xxx.x+yyy.y> N=26+28, <[DHC2006] HDF +xxx.x+yyy.y> N=6.
=E=	Catalogue in electronic form as J/ApJ/647/13
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DHC2021]
[DHC2021]	(Da Cunha+Hodge+Casey+, 2021)
Write:	<<[DHC2021] ALESSNNN 2mm.N>> <<[DHC2021] ALESSNNN_2mm.N>> (not recognised by Simbad, but found in literature)
N:	7
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band4 (2mm) continuum observations of N=7 sources. See also [HKS2013].
in source:	NAME ECDFS
Ref:	=2021ApJ...919...30D
by	DA CUNHA E. , HODGE J.A., CASEY C.M., ALGERA H.S.B., KAASINEN M., SMAIL I., WALTER F., BRANDT W.N., DANNERBAUER H., DECARLI R., GROVES B.A., KNUDSEN K.K., SWINBANK A.M., WEISS A., VAN DER WERF P., ZAVALA J.A.
	Astrophys. J., 919, 30-30 (2021)
	Measurements of the dust properties in z ≃ 1-3 submillimeter galaxies with ALMA.
o	Table 2: <[DHC2021] ALESSNNN 2mm.N> N=7.
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [DHD2013]
[DHD2013]	(D'Eugenio+Houghton+Davies+, 2013)
Write:	<<[DHD2013] NN>>
N:	30
Object:	G in ClG (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT FLAMES GIRAFFE spectroscopy of N=30 galaxies in the massive cluster A1689 at z=0.183.
in source:	ACO 1689
Ref:	=2013MNRAS.429.1258D
by	D'EUGENIO F. , HOUGHTON R.C.W., DAVIES R.L., DALLA BONTA E.
	Mon. Not. R. Astron. Soc., 429, 1258-1266 (2013)
	Fast and slow rotators in the densest environments: a FLAMES/GIRAFFE integral field spectroscopy study of galaxies in A1689 at z = 0.183.
o	(Erratum) erratum vol. 447, p. 1398 (2015)
o	Table 2: <[DHD2013] NN> (Nos 1-30).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DHD2019]
[DHD2019]	(Dannerbauer+Harrington+Diaz-Sanchez+, 2019) (Not yet in Simbad)
Write:	<<[DHD2019] CO32-A>>
N:	2
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	IRAM NOEMA CO(3-2) observations of the SMG WISE J132934.18+224327.3 revealing N=2 components.
in source:	NAME Cosmic Eyebrow
Ref:	=2019AJ....158...34D
by	DANNERBAUER H. , HARRINGTON K., DIAZ-SANCHEZ A., IGLESIAS-GROTH S., REBOLO R., GENOVA-SANTOS R.T., KRIPS M.
	Astron. J., 158, 34-34 (2019)
	Ultra-bright CO and [CI] emission in a lensed z = 2.04 submillimeter galaxy with extreme molecular gas properties.
o	HATLAS J132527+284452 (z=1.68) not identified (actually the source detected in Timmons et al. 2015 is H-ATLAS J142935.3-002836 at z=1.027).
o	Table 1: <[DHD2019] CO32-A> (Nos A to B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DHF2002]
[DHF2002]	(Duc+Hall+Fadda+, 2002)
Write:	<<[DHF2002] ISO JHHMMSS.s+DDMMSS>>
N:	1
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	Discovery of a low-ionisation BAL QSO by ISOCAM.
Ref:	=2002A&A...389L..47D
by	DUC P.-A. , HALL P.B., FADDA D., CHANIAL P., ELBAZ D., MONACO P., POMPEI E., POGGIANTI B.M., FLORES H., FRANCESCHINI A., BIVIANO A., MOORWOOD A., CESARSKY C.
	Astron. Astrophys., 389, 47-50 (2002)
	An unusual iron Lo-BAL quasar detected by ISOCAM.
o	Cluster J1888.16CL = CEMM J1888.16CL.
o	<[DHF2002] ISO J005645.1-273816> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DHG2018]
[DHG2018]	(Dekany+Hajdu+Grebel+, 2018)
Write:	<<[DHG2018] NNNN>>
N:	1892
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Stat:	is completely incorporated in Simbad
Note:	N=1892 RR Lyrae in the Southern Galactic Plane. Use of VISTA Variables in the Via Lactea (VVV) Survey data. See also [MDM2017b], [DHG2019], [DG2020].
Ref:	=2018ApJ...857...54D
by	DEKANY I. , HAJDU G., GREBEL E.K., CATELAN M., ELORRIETA F., EYHERAMENDY S., MAJAESS D., JORDAN A.
	Astrophys. J., 857, 54-54 (2018)
	A near-infrared RR Lyrae census along the southern galactic plane: the Milky Way's stellar fossil brought to light.
o	Table 1: <[DHG2018] NNNN> (Nos 1-1892).
=E=	Catalogue in electronic form as <J/ApJ/857/54/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DHG2019]
[DHG2019]	(Dekany+Hajdu+Grebel+, 2019)
Write:	<<[DHG2019] NNNN>>
N:	1294
Object:	Classical Cepheid + Type II Cepheid (SIMBAD class: Variable* = Variable Star)
Note:	N=1294 classical and type II Cepheids along the southern Galactic midplane. Use of near-infrared photometry from the VISTA Variables in the Via Lactea (VVV) survey. See also [DHG2018] and [DG2020].
Ref:	=2019ApJ...883...58D
by	DEKANY I. , HAJDU G., GREBEL E.K., CATELAN M.
	Astrophys. J., 883, 58-58 (2019)
	Into the darkness: classical and Type II Cepheids in the zona galactica incognita.
o	Table 4: <[DHG2019] NNNN> (Nos 1-1294).
=E=	Catalogue in electronic form as <J/ApJ/883/58/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DHJ2007]
[DHJ2007]	(Deng+He+Jiang+, 2007)
Write:	<<[DHJ2007] NNNNN>>
N:	11163
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	Extraction of 11163 groups of G from the SDSS DR5.
Ref:	=2007A&A...474..783D
by	DENG X.-F. , HE J.-Z., JIANG P., LUO C.-H., WU P.
	Astron. Astrophys., 474, 783-791 (2007)
	The main galaxy groups from the SDSS Data Release 5.
o	Table 2: <[DHJ2007] NNNNN> (Nos 1-11163).
=E=	Catalogue in electronic form as J/A+A/474/783
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DHK
DHK	(D.H. Kaiser)
Write:	<<DHK NN>>
N:	43
Object:	Red V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Rem:	Identif. chart.
Ref:	=1989IBVS.3313....1K
by	KAISER D.H. , WILLIAMS D.B., BALDWIN M.E.
	IAU Inform. Bull. Var. Stars, 3313, 1-4 (1989)
	Three new red variables.
o	<DHK N> (Nos 1-5).
Ref:	=1990IBVS.3442....1K
by	KAISER D.H. , BALDWIN M.E., WILLIAMS D.B.
	IAU Inform. Bull. Var. Stars, 3442, 1-4 (1990)
	Seven more undesignated variable stars.
o	<DHK NN> (Nos 6-13)
Ref:	=1990IBVS.3480....1K
by	KAISER D.H.
	IAU Inform. Bull. Var. Stars, 3480, 1-None (1990)
	Three new variable stars.
o	<DHK NN> (Nos 14-16)
Ref:	=1991IBVS.3677....1K
by	KAISER D.H.
	IAU Inform. Bull. Var. Stars, 3677, 1-None (1991)
	Eight new or undesignated variable stars.
o	<DHK NN> (Nos 17-24)
Ref:	=1992IBVS.3814....1K
by	KAISER D.H.
	IAU Inform. Bull. Var. Stars, 3814, 1-None (1992)
	Twelve new or undesignated variables.
o	<DHK NN> (Nos 25-36)
Ref:	=1994IBVS.4119....1K
by	KAISER D.H.
	IAU Inform. Bull. Var. Stars, 4119, 1-2 (1994)
	Five new DHK variables.
o	<DHK NN> (Nos 37-41)
Ref:	=1995IBVS.4274....1K
by	KAISER D.H.
	IAU Inform. Bull. Var. Stars, 4274, 1-2 (1995)
	Two new variable stars.
o	<DHK NN> (Nos 42-43)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DHL2017]
[DHL2017]	(Dapra+Henkel+Levshakov+, 2017)
Write:	<<[DHL2017] L1498-N>>
N:	2
Object:	CH3OH Em. Peak (SIMBAD class: denseCore = Dense Core)
Note:	IRAM 30m telescope EMIR observations of N=2 methanol emission peaks in LDN 1498.
in source:	LDN 1498
Ref:	=2017MNRAS.472.4434D
by	DAPRA M. , HENKEL C., LEVSHAKOV S.A., MENTEN K.M., MULLER S., BETHLEM H.L., LEURINI S., LAPINOV A.V., UBACHS W.
	Mon. Not. R. Astron. Soc., 472, 4434-4443 (2017)
	Testing the variability of the proton-to-electron mass ratio from observations of methanol in the dark cloud core L1498.
o	Table 1: <[DHL2017] L1498-N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DHM
DHM	(Durham obs.)
Write:	<<DHM HHMM+DDd>>
N:	1
Object:	QSO (SIMBAD class: QSO = Quasar)
Note:	N=1 QSO 0054-284
Ref:	=1983Natur.303..156S
by	SHANKS T. , FONG R., BOYLE B.J.
	Nature, 303, 156-158 (1983)
	Discovery of DHM 0054-284, a quasar of redshift 3.61.
o	<DHM HHMM-DDd> N=1: DHM 0054-284
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DHM2014]
[DHM2014]	(Delaye+Huertas-Company+Mei+, 2014)
Write:	<<[DHM2014] NNNN>>
N:	313
Object:	G (SIMBAD class: Galaxy)
Note:	N=313 early-type galaxies in nine massive clusters. Use of HST ACS and ESO HAWK-I Cluster Survey (HCS) data.
Ref:	=2014MNRAS.441..203D
by	DELAYE L. , HUERTAS-COMPANY M., MEI S., LIDMAN C., LICITRA R., NEWMAN A., RAICHOOR A., SHANKAR F., BARRIENTOS F., BERNARDI M., CERULO P., COUCH W., DEMARCO R., MUNOZ R., SANCHEZ-JANSSEN R., TANAKA M.
	Mon. Not. R. Astron. Soc., 441, 203-223 (2014)
	Larger sizes of massive quiescent early-type galaxies in clusters than in the field at 0.8 < z < 1.5.
o	Table B1: <[DHM2014] NNNN> N=313 among (Nos 157-4319).
=E=	Catalogue in electronic form as J/MNRAS/441/203
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DHM2015]
[DHM2015]	(Dressler+Henry+Martin+, 2015) (Not yet in Simbad)
Write:	<<[DHM2015] NN>>
N:	13
Object:	LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	Magellan-Baade Telescope IMACS and Keck DEIMOS spectroscopic observations of N=13 Lymanα emitters (LAEs) at z=5.7.
Ref:	=2015ApJ...806...19D
by	DRESSLER A. , HENRY A., MARTIN C.L., SAWICKI M., McCARTHY P., VILLANEUVA E.
	Astrophys. J., 806, 19 (2015)
	Confirmation of a steep luminosity function for Lyα emitters at z = 5.7: a major component of reionization.
o	Table 1: <[DHM2015] NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DHM99]
[DHM99]	(Dominici+Horvath+Medina Tanco+, 1999)
Write:	<<[DHM99] AANNNN>>
N:	479
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	N=479 variable stars for the 12 low-extinction windows (T.1) towards the Galactic Bulge. In the format 'AA' represent the window, and 'NNNN' a sequential counter number. See also [DTH99], objects coming from the same database of N=124976 objects.
in source:	NAME Galactic Bulge
Ref:	=1999A&AS..139..321D
by	DOMINICI T.P. , HORVATH J.E., MEDINA TANCO G.A., TEIXEIRA R., BENEVIDES-SOARES P.
	Astron. Astrophys., Suppl. Ser., 139, 321-334 (1999)
	Stellar variability in low-extinction regions towards the Galactic Bulge.
o	Table: <[DHM99] AANNNN> N=479.
=E=	Catalogue in electronic form as J/A+AS/139/321
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DHS2014]
[DHS2014]	(Da Costa+Held+Saviane+, 2014)
Write:	<<[DHS2014] NNNNNNNN>>
N:	190
Object:	RGB* + AGB* + * (SIMBAD class: Star)
Note:	VLT FORS2 and Gemini-S GMOS-S multi-object spectroscopy of N=190 stars in the field of the Galactic halo globular cluster NGC 5824.
in source:	NGC 5824
Ref:	=2014MNRAS.438.3507D
by	DA COSTA G.S. , HELD E.V., SAVIANE I.
	Mon. Not. R. Astron. Soc., 438, 3507-3520 (2014)
	NGC 5824: a luminous outer halo globular cluster with an intrinsic abundance spread.
o	Table 1: <[DHS2014] NNNNNNNN> N=190 among (Nos 11000467-72005459).
=E=	Catalogue in electronic form as J/MNRAS/438/3507
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DHT
DHT	(De Vries+Heithausen+Thaddeus)
*****	Avoid the usage of DHT, prefer VHT
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: DHW
DHW	(Dengel+Hartl+Weinberger)= (DeHt)
Write:	<<DHW 1-N>>
N:	2
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	DHW 1-1 = PK 19-13 1 = PN G019.4-13.6 DHW 1-2 = PK 11+17 1 possible PN named 'DHW 1' in Acker+ 1992ESOPN...1....1A catalogue of PN) See also 'PN DeHt N', 1980A&A....85..356D
Ref:	=1979MitAG..45..182D
by	DENGEL J. , HARTL H., WEINBERGER R.
	Mitt. Astron. Gesellschaft, 45, 182-185 (1979)
	Das Innsbrucker Poss-Durchmusterungsprogramm.
o	<DHW 1-N> (Nos 1-1, 1-2)
Origin	of the Acronym: L (1992ESOPN...1....1A)
Details on Acronym: DHW
DHW	(Dengel+Hartl+Weinberger)
*****	Avoid the usage of DHW, prefer DeHt
Origin	of the Acronym: L = Found in the literature
Details on Acronym: DI
DI	(Demers+Irwin)
*****	Avoid the usage of DI, prefer [DI87]
Origin	of the Acronym: L (2002AJ....123..840B)
Details on Acronym: DI
DI	(Demers+Irwin)
*****	Avoid the usage of DI, prefer [DI91]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DI
DI	(Demers+Irwin)
*****	Avoid the usage of DI, prefer [DI93]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [DI87]
[DI87]	(Demers+Irwin, 1987)= (DI)
Write:	<<[DI87] VNN>>
N:	30
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
in source:	NAME Fornax Dwarf Galaxy
Ref:	=1987MNRAS.226..943D
by	DEMERS S. , IRWIN M.J.
	Mon. Not. R. Astron. Soc., 226, 943-961 (1987)
	The long-period variables of Fornax - I. Search, discovery and periods.
o	in ref list SAHA 1986AJ.....92..302S instead of AJ.93
o	Table 3: <[DI87] VNN> (Nos V1-V30).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DI91]
[DI91]	(Demers+Irwin, 1991)= DI
Write:	<<[DI91] NNNN>>
N:	1679
Object:	Blue * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	Magellanic Clouds:Magellanic Bridge = Magellanic Bridge
Ref:	=1991A&AS...91..171D
by	DEMERS S. , IRWIN M.J.
	Astron. Astrophys., Suppl. Ser., 91, 171-182 (1991)
	Catalogue of blue stars between the Magellanic Clouds.
o	Table 4:<[DI91] NNNN> (Nos 1-1679)
=E=	Catalogue in electronic form as J/A+AS/91/171
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DI93]
[DI93]	(Demers+Irwin, 1993)= (DI)
Write:	<<[DI93] NNNN>> <<[DI93] VNN>>
N:	2039+80
Object:	* (SIMBAD class: Star)
Note:	Table 3: brightest stars among the 3366 identified. Maps Fig.3. Fig.2: N=80 variable-star candidates.
in source:	UGC 6253 = Leo II
Ref:	=1993MNRAS.261..657D
by	DEMERS S. , IRWIN M.J.
	Mon. Not. R. Astron. Soc., 261, 657-673 (1993)
	Deep CCD photometry of the dwarf spheroidal galaxy Leo II.
o	Table 4: ALW Leo II 1 to 7.
o	Table 3: <[DI93] NNNN> N=2039 among (Nos 1-3366). Fig.2: <[DI93] VNN> (Nos V1-V80).
=E=	Catalogue in electronic form as J/MNRAS/261/657
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DIA
DIA	(Difference Image Analysis survey)
Write:	<<DIA FFF.NNNNN.NNNN>>
N:	83
Object:	Microlensing Event (SIMBAD class: LensingEv = (Micro)Lensing Event)
Note:	See also MACHO.
Ref:	=2000ApJ...541..734A
by	ALCOCK C. , ALLSMAN R.A., ALVES D.R., AXELROD T.S., BECKER A.C., BENNETT D.P., COOK K.H., DRAKE A.J., FREEMAN K.C., GEHA M., GRIEST K., LEHNER M.J., MARSHALL S.L., MINNITI D., NELSON C.A., PETERSON B.A., POPOWSKI P., PRATT M.R., QUINN P.J., STUBBS C.W., SUTHERLAND W., TOMANEY A.B., VANDEHEI T., WELCH D.L.
	Astrophys. J., 541, 734-766 (2000)
	The MACHO project: microlensing optical depth toward the Galactic Bulge from difference image analysis.
o	(Erratum) Erratum vol. 557, p. 1035 (2001)
o	Table 4, col(1): <MACHO YY-BLG-dNN>, <MACHO YY-BLG-sNN> N=38+7. Table 4, col(2): <DIA FFF.NNNNN.NNNN> N=83.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Dias
Dias	(Dias)
Write:	<<Cl Dias NN>>
N:	11
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	From a private communication of Dias. Some Dias clusters are found in 2002A&A...389..871D.
Auth.:	DIAS W.S.
=E=	Catalogue in electronic form as B/ocl
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DIB2012]
[DIB2012]	(Dirienzo+Indebetouw+Brogan+, 2012)
Write:	<<[DIB2012] GLLL.ll+BB.bb>> <<[DIB2012] MLLL.llll+BB.bbbb>>
N:	6+58
Object:	HII + YSO (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	N=58 YSOs ("manually identified") in 6 HII regions. Use of Spitzer Space Telescope data (including the GLIMPSE Point Source Catalog).
Ref:	=2012AJ....144..173D
by	DIRIENZO W.J. , INDEBETOUW R., BROGAN C., CYGANOWSKI C.J., CHURCHWELL E., FRIESEN R.K.
	Astron. J., 144, 173 (2012)
	Testing triggered star formation in six H II regions.
o	Fig. 1, Table 1: <[DIB2012] GLLL.ll+BB.bb> N=6. Table 4: <[DIB2012] MLLL.llll+BB.bbbb> N=58.
=E=	Catalogue in electronic form as <J/AJ/144/173/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Dickinson
Dickinson	(Dickinson)
====>	Equivalent to: HNM
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DIG
DIG	(Diffuse Ionized Gas) (Not yet in Simbad)
*****	Avoid the usage of DIG, prefer [HP2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DIG
DIG	(Diffuse Ionised Gas)
*****	Avoid the usage of DIG, prefer [HS2000b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Digel
Digel	(Digel+)
*****	Avoid the usage of Digel, prefer [DDT94]
Origin	of the Acronym: L (2008ApJ...675..443Y)
Details on Acronym: DIK
DIK	(Demers+Irwin+Kunkel)= ([DIK93])
Write:	<<DIK NNa>>
N:	58
Object:	Very Red * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 1: (Nos 1-43) betw. MC. Table 2: (Nos 44-57) in the NE halo of SMC. See also [KID97], [KDI2000] Identif. charts
in source:	Magellanic Clouds:LMC = LMC
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1993MNRAS.260..103D
by	DEMERS S. , IRWIN M.J., KUNKEL W.E.
	Mon. Not. R. Astron. Soc., 260, 103-110 (1993)
	Very red stars between the Magellanic Clouds : discovery of carbon stars in the outer LMC and SMC haloes.
o	Tables 1, 2: <DIK NNa> (Nos 1-57, 8a>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DIK93]
[DIK93]	(Demers+Irwin+Kunkel, 1993)
*****	Avoid the usage of [DIK93], prefer DIK
Origin	of the Acronym: L (1997A&AS..122..463K)
Details on Acronym: DIL
DIL	(Duerr+Imhoff+Lada)
Write:	<<DIL NN>>
N:	99
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Ref:	=2000PASA...17..227D
by	DRINKWATER M.J. , JONES J.B., GREGG M.D., PHILLIPPS S.
	Publications - Astron. Soc. Australia, 17, 227-233 (2000)
	Compact stellar systems in the Fornax Cluster : super-massive star clusters or extremely compact dwarf galaxies?
o	Table 1: <[DJG2000] UCO N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DIM97]
[DIM97]	(De Mello+Infante+Menanteau, 1997)
Write:	<<[DIM97] JHHMMSS.ss+DDMMSS.s>>
N:	3632+11297
Object:	G in Pair and in Group (SIMBAD class: GinPair = Galaxy in Pair of Galaxies)
Ref:	=1997ApJS..108...99D
by	DE MELLO D.F. , INFANTE L., MENANTEAU F.
	Astrophys. J., Suppl. Ser., 108, 99-153 (1997)
	A catalog of faint interacting galaxies in pairs and groups.
o	(Erratum) Erratum vol. 111, p. 467
o	Tables 1, 2: Authors use in this paper a format 'NNNN' for the pairs and the groups, but not in 1997ApJS..110..227D. So we don't use the acronym '[DIM97a]' in SIMBAD.
o	Tables 1, 2: <[DIM97] JHHMMSS.ss+DDMMSS.s> N=1751x2+27x4+2x5+3x6. Table 1: <[DIM97a] PairG NNNN> (Nos 1-1751), <[DIM97a] GinPair NNNNA>. Table 2: <[DIM97a] GroupG NN>, <[DIM97a] GinGroup NNA>
Ref:	=1997ApJS..110..227D
by	DE MELLO D.F. , INFANTE L., MENANTEAU F., VIEIRA G.
	Astrophys. J., Suppl. Ser., 110, 227-285 (1997)
	A catalog of faint interacting galaxies in pairs and groups. II.
o	Tables 2, 3: <[DIM97] JHHMMSS.ss+DDMMSS.s> N=11297
=E=	Catalogue in electronic form as VII/205
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DIM97a]
[DIM97a]	(De Mello+Infante+Menanteau, 1997) (Not yet in Simbad)
Write:	<<[DIM97a] PairG NNNN>> <<[DIM97a] GinPair NNNNA>> <<[DIM97a] GroupG NN>> <<[DIM97a] GinGroup NNA>>
N:	1751+1751x2+29+130
Object:	Pair of G + Group of G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	1997ApJS..108...99D: The authors use the format 'NNNN' in this catalogue for the pairs and the groups. Table 1: N=1751 pairs of galaxies and 1741x2 galaxies in pair Table 2: N=30 groups of galaxies, (Nos 1-27) are quartets of galaxies, (Nos 28-29) are quintuplet See also [DIM97]
Ref:	=1997ApJS..108...99D
by	DE MELLO D.F. , INFANTE L., MENANTEAU F.
	Astrophys. J., Suppl. Ser., 108, 99-153 (1997)
	A catalog of faint interacting galaxies in pairs and groups.
o	(Erratum) Erratum vol. 111, p. 467
o	Tables 1, 2: Authors use in this paper a format 'NNNN' for the pairs and the groups, but not in 1997ApJS..110..227D. So we don't use the acronym '[DIM97a]' in SIMBAD.
o	Tables 1, 2: <[DIM97] JHHMMSS.ss+DDMMSS.s> N=1751x2+27x4+2x5+3x6. Table 1: <[DIM97a] PairG NNNN> (Nos 1-1751), <[DIM97a] GinPair NNNNA>. Table 2: <[DIM97a] GroupG NN>, <[DIM97a] GinGroup NNA>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DIR
DIR	(Diffuse IR)
Write:	<<DIR LLL+BB>>
N:	81
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Table 4: In the format, rounded galactic coordinates 'LLL+BB', with a wrong declination sign for some objects. (the proper declination sign is the one in column b)
Ref:	=1998ApJ...507..507R
by	REACH W.T. , WALL W.F., ODEGARD N.
	Astrophys. J., 507, 507-525 (1998)
	Infrared excess and molecular clouds: a comparison of new surveys of far-infrared and H I 21 centimeter emission at high galactic latitudes.
o	t.3 : R Cor Bor not identified; some object names in Table 4 are erroneous (wrong declination sign). In SIMBAD the proper declination, found in column b, is used in the object name.
o	Table 4: <DIR LLL+BB> N=81.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DIRBE
DIRBE	(Diffuse IR Background Experiment)
Write:	<<DIRBE DHHMMSSssPHHMMSSs>> <<DIRBE DHHMMSSssMHHMMSSs>>
N:	11788
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Point source catalogue of the Diffuse IR Background Experiment (DIRBE) on the Cosmic Bacground Explorer (COBE). Coordinates in the format are J2000 epoch coordinates.
Ref:	=2004ApJS..154..673S
by	SMITH B.J. , PRICE S.D., BAKER R.I.
	Astrophys. J., Suppl. Ser., 154, 673-704 (2004)
	The COBE DIRBE point source catalog.
o	Table 1: Coordinates in the format are J2000 /session define format EPOCH1 = coordinates.
o	Table 1: <DIRBE DHHMMSSssPHHMMSSs>, <DIRBE DHHMMSSssMHHMMSSs>, N=11788.
=E=	Catalogue in electronic form as J/ApJS/154/673
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DIRECT
DIRECT	(DIRECT survey, in M 31)
*****	Avoid the usage of DIRECT, prefer D31
Origin	of the Acronym: L (2007AJ....134.2474M)
Details on Acronym: DIRECT
DIRECT	(DIRECT survey, in M 33)
*****	Avoid the usage of DIRECT, prefer D33
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DIRECT
DIRECT	(DIRECT survey)
Write:	<<DIRECT VNNNNN M31A>> <<DIRECT VNNNNN M33A>>
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	DIRECT project, to obtain the direct distances to M 31 and M 33, using detached eclipsing binaries and Cepheids. After discussion with authors: Format 'VNNNNN DNNA', letter 'D' for DIRECT project, not used in SIMBAD. Format 'VNNNNN MNNA', in SIMBAD: letter 'V' for variable, 'NNNNN' for the number of the star in the database, followed by the name of the field: M31A, M31B, M31C, M31D, M31F.
in source:	M 31 = NGC 224
Ref:	=1998AJ....115.1016K
by	KALUZNY J. , STANEK K.Z., KROCKENBERGER M., SASSELOV D.D., TONRY J.L., MATEO M.
	Astron. J., 115, 1016-1044 (1998)
	DIRECT distances to nearby galaxies using detached eclipsing binaries and cepheids. I. Variables in the field M31B.
o	The format is VNNNNN DNNA in the paper (D for DIRECT), and VNNNNN MNNA in SIMBAD, after discussion with the authors.
o	Tables 1, 2, 3, 4: <DIRECT VNNNN M31B> N=85
Ref:	=1998AJ....115.1894S
by	STANEK K.Z. , KALUZNY J., KROCKENBERGER M., SASSELOV D.D., TONRY J.L., MATEO M.
	Astron. J., 115, 1894-1915 (1998)
	DIRECT distances to nearby galaxies using detached eclipsing binaries and cepheids. II. Variables in the field M31A.
o	Tables 1, 2, 3, 4: <DIRECT VNNNN M31A> N=75.
Ref:	=1999AJ....117.2810S
by	STANEK K.Z. , KALUZNY J., KROCKENBERGER M., SASSELOV D.D., TONRY J.L., MATEO M.
	Astron. J., 117, 2810-2830 (1999)
	DIRECT distances to nearby galaxies using detached eclipsing binaries and cepheids. III. Variables in the field M31C.
o	Tables 1-4: <DIRECT VNNNN M31C> N=115.
Ref:	=1999AJ....118..346K
by	KALUZNY J. , MOCHEJSKA B.J., STANEK K.Z., KROCKENBERGER M., SASSELOV D.D., TONRY J.L., MATEO M.
	Astron. J., 118, 346-365 (1999)
	DIRECT distances to nearby galaxies using detached eclipsing binaries and cepheids. IV. Variables in the field M31D.
o	Tables 1-4: <DIRECT VNNNN M31D> N=71.
Ref:	=1999AJ....118.2211M
by	MOCHEJSKA B.J. , KALUZNY J., STANEK K.Z., KROCKENBERGER M., SASSELOV D.D.
	Astron. J., 118, 2211-2228 (1999)
	DIRECT distances to nearby galaxies using detached eclipsing binaries and cepheids. V. Variables in the field M31F.
o	Misprint: inversion of Field II and III
o	Tables 1-4: <DIRECT VNNNN M31F> N=64.
=E=	Catalogue in electronic form as J/AJ/115/1016
=E=	Catalogue in electronic form as J/AJ/115/1894
=E=	Catalogue in electronic form as J/AJ/118/346
=E=	Catalogue in electronic form as J/AJ/118/2211
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DIV2015]
[DIV2015]	(De Gasperin+Intema+Van Weeren+, 2015)
Write:	<<[DIV2015] RGN>> <<[DIV2015] RG6 lobe W>> <<[DIV2015] RG6 core>> <<[DIV2015] Relic W>>
N:	9+2
Object:	Radio G + Rad (SIMBAD class: Radio = Radio Source)
Note:	GMRT 147, 323 and 607MHz and WSRT 1380MHz observations of N=9 radio galaxies in the field of PSZ1 G108.18-11.53.
in source:	PSZ1 G108.18-11.53
Ref:	=2015MNRAS.453.3483D
by	DE GASPERIN F. , INTEMA H.T., VAN WEEREN R.J., DAWSON W.A., GOLOVICH N., WITTMAN D., BONAFEDE A., BRUGGEN M.
	Mon. Not. R. Astron. Soc., 453, 3483-3498 (2015)
	A powerful double radio relic system discovered in PSZ1 G108.18-11.53: evidence for a shock with non-uniform Mach number?
o	Table 3: <[DIV2015] Relic W> (Nos N and S). Table 4: <[DIV2015] RGN> (Nos RG1-RG5, RG7), <[DIV2015] RG6 core> N=1, <[DIV2015] RG6 lobe W> (Nos N and S).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DJ
DJ	(Davidge+Jones)
Write:	<<DJ NNN>>
N:	251
Object:	* in Holmberg IX (SIMBAD class: Star)
in source:	Holmberg IX
Ref:	=1989AJ.....97.1607D
by	DAVIDGE T.J. , JONES J.H.
	Astron. J., 97, 1607-1613 (1989)
	The evolved stellar content of Holmberg IX.
o	<DJ NNN> N=251
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [DJ2014]
[DJ2014]	(Dehghan+Johnston-Hollitt, 2014)
Write:	<<[DJ2014] NN>>
N:	62
Object:	Overdensity (SIMBAD class: GroupG = Group of Galaxies)
Note:	N=62 filaments, groups, and clusters in the Chandra Deep Field South (CDFS). Use of MUSYC and ACES (Arizona CDFS Environment Survey) data.
in source:	NAME CDFS
Ref:	=2014AJ....147...52D
by	DEHGHAN S. , JOHNSTON-HOLLITT M.
	Astron. J., 147, 52 (2014)
	Clusters, groups, and filaments in the Chandra Deep Field-South up to redshift 1.
o	Table 2: <[DJ2014] NN> (Nos 1-62).
=E=	Catalogue in electronic form as <J/AJ/147/52/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DJC2017]
[DJC2017]	(Dehghan+Johnston-Hollitt+Colless+, 2017)
Write:	<<[DJC2017] JHHMMSS.ss+DDMMSS.s>> <<[DJC2017] A3266 ID N>> <<[DJC2017] A3266 WCC>> <<[DJC2017] A3266 WWS>>
N:	1303+6+2+2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	AAT 2dF spectroscopic observations of N=1303 galaxies, N=6 groups of galaxies and N=4 sub-structures of the galaxy cluster Abell 3266.
in source:	ACO 3266
Ref:	=2017MNRAS.468.2645D
by	DEHGHAN S. , JOHNSTON-HOLLITT M., COLLESS M., MILLER R.
	Mon. Not. R. Astron. Soc., 468, 2645-2654 (2017)
	Dynamics of Abell 3266 - I. An optical view of a complex merging cluster.
o	Table 2: <[DJC2017] JHHMMSS.ss+DDMMSS.s> N=1303. Table 3: <[DJC2017] A3266 ID N> (Nos 1-6), <[DJC2017] A3266 WCC> N=2 (Nos WCC and ECC), <[DJC2017] A3266 WWS> N=2 (Nos NWS and SES).
=E=	Catalogue in electronic form as J/MNRAS/468/2645
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DJF2005]
[DJF2005]	(David+Jones+FOrman+, 2005)
Write:	<<[DJF2005] NN>>
N:	66
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of NGC 3379.
in source:	NGC 3379
Ref:	=2005ApJ...635.1053D
by	DAVID L.P. , JONES C., FORMAN W., MURRAY S.S.
	Astrophys. J., 635, 1053-1061 (2005)
	The diffuse emission and a variable ultraluminous X-ray point source in the elliptical galaxy NGC 3379.
o	In title and fig.1, ULX = [SGT2004] J104750.00+123456.9, fig.6 : S1, S2 = [WFB2003] 48, 53
o	Table 1: <[DJF2005] NN> (Nos 1-66).
=E=	Catalogue in electronic form as J/ApJ/635/1053
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DJF2014]
[DJF2014]	(Dehghan+Johnston-Hollitt+Franzen+, 2014)
Write:	<<[DJF2014] NN>>
N:	56
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=56 extended radio sources in the Chandra Deep Field South. Use of ATLAS (DR1 and DR3) 1.4GHz data.
in source:	NAME CDFS
Ref:	=2014AJ....148...75D
by	DEHGHAN S. , JOHNSTON-HOLLITT M., FRANZEN T.M.O., NORRIS R.P., MILLER N.A.
	Astron. J., 148, 75 (2014)
	Bent-tailed radio sources in the Australia Telescope Large Area Survey of the Chandra Deep Field-South.
o	APMCC 40 is a misprint for APMCC 401. The galaxy group MZ 00108 is not in Simbad (not enough information).
o	Fig. 1, Table 1: <[DJF2014] NN> (Nos 1-56).
=E=	Catalogue in electronic form as <J/AJ/148/75/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DJG2000]
[DJG2000]	(Drinkwater+Jones+Gregg+, 2000)= (UCD) = (UCO)
Write:	<<[DJG2000] UCO NN>>
N:	27
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Ultra Compact Objects (UCO in the format) dwarf galaxies in the Fornax Cluster. See also FCOS, [GDE2009].
in source:	NAME Fornax Cluster
Ref:	=2000PASA...17..227D
by	DRINKWATER M.J. , JONES J.B., GREGG M.D., PHILLIPPS S.
	Publications - Astron. Soc. Australia, 17, 227-233 (2000)
	Compact stellar systems in the Fornax Cluster : super-massive star clusters or extremely compact dwarf galaxies?
o	Table 1: <[DJG2000] UCO N> (Nos 1-5).
Ref:	=2003MNRAS.344..188K
by	KARICK A.M. , DRINKWATER M.J., GREGG M.D.
	Mon. Not. R. Astron. Soc., 344, 188-200 (2003)
	The surface brightness and colour-magnitude relations for Fornax cluster galaxies.
o	Fig.4, Table 4: <[DJG2000] UCO N> (Nos 6-7) added.
Ref:	=2008AJ....136..461E
by	EVSTIGNEEVA E.A. , DRINKWATER M.J., PENG C.Y., HILKER M., DE PROPRIS R., JONES J.B., PHILLIPPS S., GREGG M.D., KARICK A.M.
	Astron. J., 136, 461-478 (2008)
	Structural properties of ultra-compact dwarf galaxies in the Fornax and Virgo clusters.
o	Table 1: <[DJG2000] UCO NN> N=11 among (Nos 16-55) added.
Ref:	=2008A&A...489.1023M
by	MIESKE S. , HILKER M., BOMANS D.J., REY S.-C., KIM S., YOON S.-J., CHUNG C.
	Astron. Astrophys., 489, 1023-1028 (2008)
	Compact stellar systems in the Fornax cluster: a UV perspective.
o	Table 1: UCDk and UCDm = FCOS 3-2037 and FCOS 2-2153 respectively.
o	Tables 1,2: <[DJG2000] UCO NN> N=9 among (Nos 12-39). Tables 1,2: <[MHB2008] KNNNN> N=4, <[MHB2008] YNNNNN> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DJG2003]
[DJG2003]	(Doherty+Johnston+Green+, 2003) (Not yet in Simbad)
Write:	<<[DJG2003] Na>>
N:	7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Fig.2: N=7 unresolved sources, possible counterparts of 3EG J1410-6147.
Ref:	=2003MNRAS.339.1048D
by	DOHERTY M. , JOHNSTON S., GREEN A.J., ROBERTS M.S.E., ROMANI R.W., GAENSLER B.M., CRAWFORD F.
	Mon. Not. R. Astron. Soc., 339, 1048-1056 (2003)
	A search for the radio counterpart of the unidentified γ-ray source 3EG J1410-6147.
o	Fig.2: <[DJG2003] Na> (Nos 1, 2a-2b, 3-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DJK2020]
[DJK2020]	(Dai+Johnston+Kerr+, 2020)
Write:	<<[DJK2020] NN>>
N:	14
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA 2.1GHz continuum observations of N=14 sources in the core region of ω Cen.
in source:	NGC 5139 = ome Cen
Ref:	=2020ApJ...888L..18D
by	DAI S. , JOHNSTON S., KERR M., CAMILO F., CAMERON A., TOOMEY L., KUMAMOTO H.
	Astrophys. J., 888L, 18-18 (2020)
	Discovery of millisecond pulsars in the globular cluster Omega Centauri.
o	Table 1: <[DJK2020] NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DJM
DJM	(D.J. McConnell)
Write:	<<DJM NNN>>
N:	466
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Ref:	=1988AJ.....96..354M
by	MacCONNELL D.J.
	Astron. J., 96, 354-364 (1988)
	New galactic carbon stars found on southern, near-infrared spectrum plates.
o	Table I: <DJM NNN> (Nos 1-466)
=E=	Catalogue in electronic form as <III/132/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Djorg
Djorg	(Djorgovski)= (Djorgovski)
Write:	<<Cl Djorg N>>
N:	3
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Ref:	=1987ApJ...317L..13D
by	DJORGOVSKI S.
	Astrophys. J., 317, 13-14 (1987)
	Discovery of three obscured globular clusters.
o	<Cl Djorg N> (Nos 1-3)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Djorgovski
Djorgovski	(Djorgovski)
====>	Equivalent to: Djorg
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [DJS2015]
[DJS2015]	(Dawson+Jee+Stroe+, 2015)
Write:	<<[DJS2015] JHHMMSS.sss+DDMMSS.sss>>
N:	428
Object:	G (SIMBAD class: Galaxy)
Note:	Keck DEIMOS spectroscopic observations of N=441 galaxies in the field of the merging cluster CIZA J2242.8+5301.
in source:	CIZA J2242.8+5301
Ref:	=2015ApJ...805..143D
by	DAWSON W.A. , JEE M.J., STROE A., NG Y.K., GOLOVICH N., WITTMAN D., SOBRAL D., BRUGGEN M., ROTTGERING H.J.A., VAN WEEREN R.J.
	Astrophys. J., 805, 143 (2015)
	MC^{2}: galaxy imaging and redshift analysis of the merging cluster CIZA J2242.8+5301.
o	Table 1: <[DJS2015] JHHMMSS.sss+DDMMSS.sss> N=441.
=E=	Catalogue in electronic form as J/ApJ/805/143
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DJT2019]
[DJT2019]	(Denes+Jones+Toth+, 2019)
Write:	<<[DJT2019] JHHMMSS+DDMMSS>>
N:	10
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA 1.4GHz continuum observations of N=10 radio continuum sources in the fields of GRB 070508, GRB 081008, GRB 100621A. Use of data from the Galactic All Sky Survey (GASS), and data from the Planck Legacy Archive and from the Swift archive.
Ref:	=2019MNRAS.489.3778D
by	DENES H. , JONES P.A., TOTH L.V., ZAHORECZ S., KOO B.-C., PINTER S., RACZ I.I., BALAZS L.G., CUNNINGHAM M.R., DOI Y., HORVATH I., KOVACS T., ONISHI T., SULEIMAN N., BAGOLY Z.
	Mon. Not. R. Astron. Soc., 489, 3778-3796 (2019)
	Exploring the pattern of the Galactic H I foreground of GRBs with the ATCA.
o	Table 3: <[DJT2019] JHHMMSS+DDMMSS> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DJW84]
[DJW84]	(Dreher+Johnston+Welch+, 1984)
Write:	<<[DJW84] W49 AN>> <<[DJW84] W49 ANa>> <<[DJW84] W49 AA>> <<[DJW84] W49 AAw>> <<[DJW84] W49S-1>>
N:	19+39
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Components of W 49 (sometimes cited as components of W 49N): N=19 (Nos A-S), N=18 subcomponents with a format 'AN', and N=4 'ANa', the component G1S (South of G1) is G1s in SIMBAD. N=12 new components with a format 'AA', and N=4 'AAw'. A Component in the South region, format 'W49S-1' is also added. See also CB01.
in source:	W 49:W 49A = W 49A
Ref:	=1984ApJ...283..632D
by	DREHER J.W. , JOHNSTON K.J., WELCH W.J., WALKER R.C.
	Astrophys. J., 283, 632-639 (1984)
	Ultracompact structure in the HII region W 49N.
o	Table 1: <[DJW84] W49 AN> (Nos A-G), (Nos G1-G2).
Ref:	=1990ApJ...351..189D
by	DICKEL H.R. , GOSS W.M.
	Astrophys. J., 351, 189-205 (1990)
	VLA observations of the 6 centimeter and 2 centimeter lines of H2CO in the direction of W 49.
o	Table 2: <[DJW84] W49 A> (Nos H-S) added.
Ref:	=1997ApJ...482..307D
by	DE PREE C.G. , MEHRINGER D.M., GOSS W.M.
	Astrophys. J., 482, 307-333 (1997)
	Multifrequency, high-resolution radio recombination line observations of the massive star-forming region W49A.
o	Table 4: <[DJW84] W49 AN> N=11 added, <[DJW84] W49 AA> N=11, <[DJW84] W49S-1) N=1.
Ref:	=2000ApJ...540..308D
by	DE PREE C.G. , WILNER D.J., GOSS W.M., WELCH W.J., McGRATH E.
	Astrophys. J., 540, 308-315 (2000)
	Ultracompact H II regions in W49N at 500 AU scales: shells, winds, and the water maser source.
o	Fig.2, Table 3: <[DJW84] W49 AN> (Nos A1-A2, B2) added, <[DJW84] W49 ANa> (Nos G1a-G1c).
Ref:	=2000ApJ...540..316S
by	SMITH N. , JACKSON J.M., KRAEMER K.E., DEUTSCH L.K., BOLATTO A., HORA J.L., FAZIO G., HOFFMANN W.F., DAYAL A.
	Astrophys. J., 540, 316-331 (2000)
	Thermal infrared imaging of ultracompact H II regions in W49A.
o	Fig.3, Table 2: <[DJW84] W49 AA> (No. DD) added, <[DJW84] W49 AAw> (Nos BBe, DDs, EEe, HHw).
Ref:	=2001ApJ...550L..81W
by	WILNER D.J. , DE PREE C.G., WELCH W.J., GOSS W.M.
	Astrophys. J., 550, 81-85 (2001)
	Hot cores in W49N and the timescale for hot core evolution.
o	Fig.1: <[DJW84] W49 AN> (No. K2) added. Fig.2, Table 2: <[WDW2001] MCN a> (Nos a-f).
Ref:	=2004ApJ...600..286D
by	DE PREE C.G. , WILNER D.J., MERCER A.J., DAVIS L.E., GOSS W.M., KURTZ S.
	Astrophys. J., 600, 286-291 (2004)
	Broad recombination line objects in W49 north on 600 AU scales.
o	Table 1: Source G1S is [DJW84] W49 G1s in SIMBAD.
o	Table 1: <[DJW84] W49 ANa> (Nos B3, G1s) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DK
DK	(Demers+Kunkel)= ([DK79])
Write:	<<DK NN>>
N:	66
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Rem:	Identif. charts
in source:	NAME Fornax Dwarf Galaxy
Ref:	=1979PASP...91..761D
by	DEMERS S. , KUNKEL W.E.
	Publ. Astron. Soc. Pac., 91, 761-765 (1979)
	Discovery of very red giants in the Fornax galaxy.
o	<DK NN> N=66
Origin	of the Acronym: L = Found in the literature
Details on Acronym: DK
DK	(Demers+Kunkel)
*****	Avoid the usage of DK, prefer [DK76]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Dk
Dk	(Dark nebula)
*****	Avoid the usage of Dk, prefer [H72b]
Origin	of the Acronym: L (1988PASP..100..346H)
Details on Acronym: [DK2003]
[DK2003]	(Di Stefano+Kong, 2003)
Write:	<<[DK2003] M101-NNN>> <<[DK2003] M51-NN>> <<[DK2003] M83-NNN>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra data are used to identify luminous candidate supersoft X-ray sources in 3 external galaxies. See also [PSM2001], [SW2002b], [SW2003].
in source:	M 101 = NGC 5457
in source:	M 51 = NGC 5194
in source:	M 83 = NGC 5236
Ref:	=2003ApJ...592..884D
by	DI STEFANO R. , KONG A.K.H.
	Astrophys. J., 592, 884-899 (2003)
	Luminous supersoft X-ray sources in external galaxies.
o	In the abstract NGC 4967 is a misprint for NGC 4697. Table 3: Objects in NGC 4697 are [SIB2001] in SIMBAD.
o	Table 3: <[DK2003] M101-NNN> N=16 among (Nos 15-104), <[DK2003] M51-NN> N=4 among (Nos 12-58), <[DK2003] M83-NNN> N=10 among (Nos 20-128).
Ref:	=2004ApJ...609..710D
by	DI STEFANO R. , KONG A.K.H.
	Astrophys. J., 609, 710-727 (2004)
	The discovery of quasi-soft and supersoft sources in external galaxies.
o	In Abstract : NGC 4967 is a misprint for NGC 4697. Table 4: Sources in NGC 4697 are [SIB2001] in SIMBAD.
o	Table 1: <[DK2003] M101-NNN> N=37 added among (Nos 2-116). Table 2: <[DK2003] M83-NNN> N=44 added among (Nos 1-127). Table 3: <[DK2003] M51-NN> N=20 added among (Nos 5-70).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DK2008]
[DK2008]	(Deguchi+Koike, 2008)
Write:	<<[DK2008] CN>>
N:	5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Clustering of Meter-wave Luminous Objects (MLOs) using VLSS and NVSS data.
Ref:	=2008PASJ...60L..31D
by	DEGUCHI S. , KOIKE K.
	PASJ, 60L, 31-36 (2008)
	Clustering of meter-wave luminous objects toward Monoceros.
o	Table 1 object not in SIMBAD (speculative nature of clusters of radio source).
o	Table 1: <[DK2008] CN> (Nos C1-C5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DK2009]
[DK2009]	(Dwarakanath+Kale, 2009)
Write:	<<[DK2009] HHMMA>>
N:	10
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA 330GHz and GMRT 1290GHz observations of steep spectrum radio sources.
Ref:	=2009ApJ...698L.163D
by	DWARAKANATH K.S. , KALE R.
	Astrophys. J., 698L, 163-168 (2009)
	Relics of double radio sources.
o	In paragraph 3, 0041-0923 is not identified.
o	Table 1: <[DK2009] HHMMA> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DK2010]
[DK2010]	(Dedes+Kalberla, 2010)
Write:	<<[DK2010] GLLL.l+BB.b>>
N:	25
Object:	HI Cloud (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	Effelsberg 100m telescope, WSRT and VLA observations of Galactic HI clouds.
Ref:	=2010A&A...509A..60D
by	DEDES L. , KALBERLA P.M.W.
	Astron. Astrophys., 509A, 60-60 (2010)
	Properties of extra-planar HI clouds in the outer part of the Milky way.
o	Table 1: <[DK2010] GLLL.l+BB.b> N=25.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DK2012]
[DK2012]	(Dimitrov+Kjurkchieva, 2012) (Not yet in Simbad)
Write:	<<[DK2012] StN>> <<[DK2012] Var>>
N:	8+1
Object:	* (SIMBAD class: Star)
Note:	Rozhen National Astronomical Observatory observations of the field of 2MASS J01074282+4845188.
Ref:	=2012NewA...17...34D
by	DIMITROV D.P. , KJURKCHIEVA D.P.
	NewA, 17, 34-37 (2012)
	2MASS J01074282+4845188: a new nova-like cataclysmic star with a deep eclipse.
o	Fig. 1, Table 2: <[DK2012] StN> (Nos St1-St8), <[DK2012] Var> N=1.
o	St8 is 2MASS J01074441+4844581 and VAR is 2MASS J01074282+4845188 in SIMBAD.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DK76]
[DK76]	(Demers+Kunkel, 1976)= (DK)
Write:	<<[DK76] NNN>>
N:	184 among 497
Object:	* in Cl* (SIMBAD class: Star)
in source:	NAME Reticulum Cluster
Ref:	=1976ApJ...208..932D
by	DEMERS S. , KUNKEL W.E.
	Astrophys. J., 208, 932-943 (1976)
	The Reticulum system, an analog to the Draco dwarf galaxy near the Large Magellanic Cloud.
o	<[DK76] NNN> N=184 among 497
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DK79]
[DK79]	(Demers+Kunkel, 1979)
*****	Avoid the usage of [DK79], prefer DK
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DKB
DKB	(Dannerbauer+Kurk+De Breuck)
Write:	<<DKB NNa>> <<DKB SMM JHHMMSS.s+DDMMSS>> <<DKB SMM HHMMSS.s+DDMMSS>> (not recognised by Simbad, but found in literature)
N:	16+16+8
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	APEX LABOCA 870µm and VLA 20cm observations of N=16 sources in the field of the radio galaxy MRC 1138-262. Counterparts were found in multiwavelength archival data (Subaru MOIRCS, Herschel PACS and SPIRE, Spitzer MIPS and IRAC, deep HST, VLA 1.4GHz, VLT FORS2, ISAAC and SINFONI).
in source:	NAME Spiderweb protocluster = NAME MRC 1138-262 Protocluster
Ref:	=2014A&A...570A..55D
by	DANNERBAUER H. , KURK J.D., DE BREUCK C., WYLEZALEK D., SANTOS J.S., KOYAMA Y., SEYMOUR N., TANAKA M., HATCH N., ALTIERI B., COIA D., GALAMETZ A., KODAMA T., MILEY G., ROETTGERING H., SANCHEZ-PORTAL M., VALTCHANOV I., VENEMANS B., ZIEGLER B.
	Astron. Astrophys., 570A, 55-55 (2014)
	An excess of dusty starbursts related to the Spiderweb galaxy.
o	Table 1 col(1): <DKB SMM JHHMMSS.s+DDMMSS> N=16 = Figs 2+6, Table 1 col(2): <DKB NN> (Nos 01-16). Figs 2+6: <DKB NNa> (Nos 01a-01b, 08a-08b, 12a-12d).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DKB2014]
[DKB2014]	(Dias+Kerber+Barbuy+, 2014)= ([DKB2014a]) (Not yet in Simbad)
Write:	<<[DKB2014] JHHMMSS.ss+DDMMSS.ss>>
N:	252+2309+5457+2667+1334+2019
Object:	* (SIMBAD class: Star)
Note:	SOAR 4.1m telescope SOI observations of stars in six SMC stellar clusters.
in source:	Magellanic Clouds:SMC:Cl AM 3 = Cl AM 3
in source:	Magellanic Clouds:SMC:HW 1 = HW 1
in source:	Magellanic Clouds:SMC:HW 34 = HW 34
in source:	Magellanic Clouds:SMC:HW 40 = HW 40
in source:	Magellanic Clouds:SMC:Cl Lindsay 2 = Cl Lindsay 2
in source:	Magellanic Clouds:SMC:Cl Lindsay 3 = Cl Lindsay 3
Ref:	=2014A&A...561A.106D
by	DIAS B. , KERBER L.O., BARBUY B., SANTIAGO B., ORTOLANI S., BALBINOT E.
	Astron. Astrophys., 561A, 106-106 (2014)
	Self-consistent physical parameters for five intermediate-age SMC stellar clusters from CMD modelling.
o	am3.dat, hw1.dat, hw34.dat, hw40.dat, l2.dat, l3.dat: <[DKB2014] JHHMMSS.ss+DDMMSS.ss> N=252+2309+5457+2667+1334+2019.
=E=	Catalogue in electronic form as J/A+A/561/A106
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DKB2014a]
[DKB2014a]	(Dias+Kerber+Barbuy+, 2014) (Not yet in Simbad)
*****	Avoid the usage of [DKB2014a], prefer [DKB2014]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DKB2014b]
[DKB2014b]	(Dobrovolskas+Kucinskas+Bonifacio+, 2014)
Write:	<<[DKB2014b] NNNNNNNN>>
N:	110
Object:	* (SIMBAD class: Star)
Note:	ESO VLT GIRAFFE observations of N=110 turn-off stars in 47 Tuc.
in source:	NGC 104 = 47 Tuc
Ref:	=2014A&A...565A.121D
by	DOBROVOLSKAS V. , KUCINSKAS A., BONIFACIO P., KOROTIN S.A., STEFFEN M., SBORDONE L., CAFFAU E., LUDWIG H.-G., ROYER F., PRAKAPAVICIUS D.
	Astron. Astrophys., 565A, 121-121 (2014)
	Abundances of lithium, oxygen, and sodium in the turn-off stars of Galactic globular cluster 47 Tucanae.
o	Table A.1: <[DKB2014b] NNNNNNNN> N=110 among (Nos 6129-10000094).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [DKB98]
[DKB98]	(Djorgovski+Kulkarni+Bloom+, 1998)
Write:	<<[DKB98] G>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of GRB 980703
Ref:	=1998ApJ...508L..17D
by	DJORGOVSKI S.G. , KULKARNI S.R., BLOOM J.S., GOODRICH R., FRAIL D.A., PIRO L., PALAZZI E.
	Astrophys. J., 508, 17-20 (1998)
	Spectroscopy of the host galaxy of the γ-ray burst 980703.
o	<[DKB98] G> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DKC2000]
[DKC2000]	(Doublier+Kunth+Courbin+, 2000) (Not yet in Simbad)
Write:	<<[DKC2000] N>>
N:	3
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	N=3 blobs distinct substructures in the central part of POX 186.
in source:	POX 186
Ref:	=2000A&A...353..887D
by	DOUBLIER V. , KUNTH D., COURBIN F., MAGAIN P.
	Astron. Astrophys., 353, 887-892 (2000)
	POX 186: the ultracompact blue compact dwarf galaxy reveals its nature.
o	Table 1: <[DKC2000] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DKC2018]
[DKC2018]	(De+Kasliwal+Cantwell+, 2018)
Write:	<<[DKC2018] ObjNN>>
N:	12
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck I LRIS spectroscopic observations of N=12 galaxies in the field of the IPTF 16hgs transient. Use of archival SDSS data.
Ref:	=2018ApJ...866...72D
by	DE K. , KASLIWAL M.M., CANTWELL T., CAO Y., CENKO S.B., GAL-YAM A., JOHANSSON J., KONG A., KULKARNI S.R., LUNNAN R., MASCI F., MATUSZEWSKI M., MOOLEY K.P., NEILL J.D., NUGENT P.E., OFEK E.O., PERROTT Y., REBBAPRAGADA U.D., RUBIN A., O'SULLIVAN D., YARON O.
	Astrophys. J., 866, 72-72 (2018)
	IPTF 16hgs: a double-peaked Ca-rich gap transient in a metal-poor, star-forming dwarf galaxy.
o	Table 3: <[DKC2018] ObjNN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DKF89]
[DKF89]	(Davidson+Kinman+Friedman, 1989)
Write:	<<[DKF89] WW>> <<[DKF89] A>>
N:	2+5
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=2 Condensations 'NW' and 'SE', and N=7 regions (Nos A-G) in Zw I 18. See also [HTI2003], [VWH98]
in source:	Zw I 18 = Mrk 116
Ref:	=1989AJ.....97.1591D
by	DAVIDSON K. , KINMAN T.D., FRIEDMAN S.D.
	Astron. J., 97, 1591-1599 (1989)
	High-resolution spectroscopy and direct imaging of the dwarf galaxy I Zw 18.
o	<[DKF89] WW> (Nos NW, SE), <[DKF89] A> (Nos A-E)
Ref:	=1990ApJ...350..149D
by	DUFOUR R.J. , HESTER J.J.
	Astrophys. J., 350, 149-154 (1990)
	Extended emission and star formation in I Zw 18.
o	<[DKF89] A> (Nos F-G)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DKG2002]
[DKG2002]	(Di Stefano+Kong+Garcia+, 2002)
Write:	<<[DKG2002] NN>>
N:	28
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of M 31. N=28 X-ray sources observed in M 31 globular clusters. See also CXOM31.
in source:	M 31 = NGC 224
Ref:	=2002ApJ...570..618D
by	DI STEFANO R. , KONG A.K.H., GARCIA M.R., BARMBY P., GREINER J., MURRAY S.S., PRIMINI F.A.
	Astrophys. J., 570, 618-636 (2002)
	Bright X-ray sources in M31 globular clusters.
o	Table 3: ID Mita = [M93b] NNN in SIMBAD. Table 3 note e : Source 25 is a misprint for Source 24.
o	Table 3: <[DKG2002] NN> (Nos 1-28) = <CXOM31 JHHMMSS.s+DDMMSS> N=28.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DKG90
DKG90	(Demers+Kunkel+Grondin, 1990)
*****	Avoid the usage of DKG90, prefer [DKG90]
Origin	of the Acronym: L (1997A&A...317...54J)
Details on Acronym: [DKG90]
[DKG90]	(Demers+Kunkel+Grondin, 1990)= (Demers) = (DKG90)
Write:	<<[DKG90] NNN>>
N:	97
Object:	* in Cl* (SIMBAD class: Star)
Note:	N=97 * among (Nos 9-251) in Cluster 'Fornax 1'. Identif. chart.
in source:	NAME Fornax 1
Ref:	=1990PASP..102..632D
by	DEMERS S. , KUNKEL W.E., GRONDIN L.
	Publ. Astron. Soc. Pac., 102, 632-638 (1990)
	CCD photometry of cluster 1 of Fornax.
o	Table 2: <[DKG90] NNN> N=97 among (Nos 9-251)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DKH
DKH	(Demers+Kunkel+Hardy)
Write:	<<DKH A>> <<DKH NNNNN>>
Object:	* (SIMBAD class: Star)
Note:	reference stars in the vicinity of Fornax Dwarf galaxy. See also [VDH81]
in source:	NAME Fornax Dwarf Galaxy
Ref:	=1979ApJ...232...84D
by	DEMERS S. , KUNKEL W.E., HARDY E.
	Astrophys. J., 232, 84-90 (1979)
	The giant branch of Fornax.
o	Table 1: <DKH A> N=21 among (Nos A-X), <DKH NNNNN> N=11 among (Nos 6673-11505)
Ref:	=1981AJ.....86..357V
by	VERNER G. , DEMERS S., HARDY E., KUNKEL W.E.
	Astron. J., 86, 357-370 (1981)
	The globular clusters of Fornax.
o	Table II: <DKH NN> (Nos 8, 11, 34, 36) added. Table IV: <[VDH81] Cluster 1 NN> N=36 among 90, <[VDH81] Cluster 2 NNN> N=38 among 217, <[VDH81] CF2 NNN> N=26 among 181, <[VDH81] Cluster 3 NNN> N=43 among 170, <[VDH81] CF3 NNN> N=28 among 141, <[VDH81] Cluster 4 NN> N=9 among 50, <[VDH81] Cluster 5 NNN> N=50 among 148, <[VDH81] Cluster 6 NN> N=19 among 86.
Origin	of the Acronym: L (1980ApJ...240..804A)
Details on Acronym: DKI
DKI	(Demers+Kunkel+Irwin)= (APM)
Write:	<<DKI a>> <<DKI NNNN>> <<DKI VN>> <<DKI GNN>>
N:	16+361+6+10
Object:	* + Gl? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table II: N=16 photoelectric sequence , (Nos a-r), i, o missing. Table IV: N=361 among (Nos 1838-4146), always a 4 digit format. Table VIII: N=6 V*, (Nos V1-V6). Table IX: N=10 globular cluster candidates, (Nos G1-G10)
in source:	NGC 3109
Ref:	=1985AJ.....90.1967D
by	DEMERS S. , KUNKEL W.E., IRWIN M.J.
	Astron. J., 90, 1967-1981 (1985)
	Automated photometry of NGC 3109.
o	Table II: <DKI a> (Nos a-r) i, o missing. Table IV: <DKI NNNN> N=361 among (Nos 1838-4146). Table VIII: <DKI VN> (Nos V1-V6). Table IX: <DKI GNN> (Nos G1-G10)
Origin	of the Acronym: L (1988AJ.....96.1599S)
Details on Acronym: [DKI84]
[DKI84]	(Demers+Kibblewhite+Irwin+, 1984)
*****	Avoid the usage of [DKI84], prefer DKIB
Origin	of the Acronym: L = Found in the literature
Details on Acronym: DKIB
DKIB	(Demers+Kibblewhite+Irwin+Bunclarck or Bridgeland)= ([DKI84])
Write:	<<DKIB A>> <<DKIB NNNa>>
N:	17+231
Object:	* (SIMBAD class: Star)
Note:	Table 2: Photoelectric sequence, (Nos A-S), Nos I and O missing. Table 3: program stars.
in source:	NAME Leo A
Ref:	=1984AJ.....89.1160D
by	DEMERS S. , KIBBLEWHITE E.J., IRWIN M.J., BUNCLARK P.S., BRIDGELAND M.T.
	Astron. J., 89, 1160-1165 (1984)
	Leo A : color-magnitude diagram of its brightest stars.
o	Table 2: <DKIB A> (Nos A-S, I and O missing). Table 3: <DKIB NNNa> (Nos 1-228), N=231.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [DKM2008]
[DKM2008]	(Dawson+Kawamura+Mizuno+, 2008)
Write:	<<[DKM2008] NNNa>>
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	NANTEN 12CO(1-0) and 13CO(1-0) observations of the Carina Flare Supershell.
in source:	NAME Carina Flare Supershell
Ref:	=2008PASJ...60.1297D
by	DAWSON J.R. , KAWAMURA A., MIZUNO N., ONISHI T., FUKUI Y.
	PASJ, 60, 1297-1315 (2008)
	Catalogue of ^{12}CO(J = 1–0) and 13CO(J = 1–0) molecular clouds in the Carina flare supershell.
o	G288.5+1.5 = [GCB88] 12 ([GCB88] 288.6+1.5)
o	Tables 2-4: <[DKM2008] NNNa> N=-.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DKM2012]
[DKM2012]	(Donovan Meyer+Koda+Momose+, 2011)
Write:	<<[DKM2012] NN>>
N:	30 (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	Nobeyama 45m telescope and CARMA CO(1-0) observations of NGC 6946.
in source:	NGC 6946
Ref:	=2012ApJ...744...42D
by	DONOVAN MEYER J. , KODA J., MOMOSE R., FUKUHARA M., MOONEY T., TOWERS S., EGUSA F., KENNICUTT R., KUNO N., CARTY M., SAWADA T., SCOVILLE N.
	Astrophys. J., 744, 42 (2012)
	Resolved measurements of X_{CO} in NGC 6946.
o	Table 3: <[DKM2012] NN> (Nos 1-30)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DKM2013]
[DKM2013]	(Donovan Meyer+Koda+Momose+, 2013)
Write:	<<[DKM2013] NGC NNNN-NN>>
N:	182
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	Nobeyama 45m radio telescope and CARMA CO(1-0) observations of N=182 giant molecular clouds in the inner disks of the nearby spiral galaxies NGC 4736, NGC 4826, and NGC 6946. See also [DKM2012].
in source:	NGC 4736
in source:	NGC 4826
in source:	NGC 6946
Ref:	=2013ApJ...772..107D
by	DONOVAN MEYER J. , KODA J., MOMOSE R., MOONEY T., EGUSA F., CARTY M., KENNICUTT R., KUNO N., REBOLLEDO D., SAWADA T., SCOVILLE N., WONG T.
	Astrophys. J., 772, 107 (2013)
	Resolved giant molecular clouds in nearby spiral galaxies: insights from the CANON CO (1-0) survey.
o	Table 4: <[DKM2013] NGC NNNN-NN> (Nos NGC 4736-1 to NGC 4736-9, NGC 4826-1 to NGC 4826-86, NGC 6946-1 to NGC 6946-87).
=E=	Catalogue in electronic form as J/ApJ/772/107
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DKM97]
[DKM97]	(Davis+Keel+Mulchaey+, 1997) (Not yet in Simbad)
Write:	<<[DKM97] NGC 2276 NN>> <<[DKM97] NGC 1961 NN>> <<[DKM97] NGC 1961 Knot N>>
N:	17+32+4
Object:	HII + (Rad) (SIMBAD class: HIIReg = HII Region)
Note:	Table 3: N=17 HII regions in NGC 2276, format 'NGC 2276 NN'. N=32 HII regions in NGC 1961, format 'NGC 1961 NN'. Fig.5: N=4 radio knots in NGC 1961, format 'NGC 1961 Knot N'
in source:	NGC 2276
in source:	NGC 1961
Ref:	=1997AJ....114..613D
by	DAVIS D.S. , KEEL W.C., MULCHAEY J.S., HENNING P.A.
	Astron. J., 114, 613-625 (1997)
	Gravitational interactions in poor galaxy groups.
o	Table 3: <[DKM97] NGC 2276 NN> (Nos 1-17), <[DKM97] NGC 1961 NN> (Nos 1-32). Fig.5: <[DKM97] NGC 1961 Knot N> (Nos 1-4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DKP2011]
[DKP2011]	(Durant+Kargaltsev+Pavlov+, 2011)
Write:	<<[DKP2011] A>>
N:	9
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST observations of the field of SGR 0418+5729.
Ref:	=2011ApJ...742...77D
by	DURANT M. , KARGALTSEV O., PAVLOV G.G.
	Astrophys. J., 742, 77 (2011)
	Search for the optical counterpart to Sgr 0418+5729.
o	Fig. 1, Table 1: <[DKP2011] A> (Nos A-I).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DKP87]
[DKP87]	(Dickey+Keller+Pennington+, 1987)
Write:	<<[DKP87] HHMMSS.ss+DDMMSS.s>>
N:	667
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	NAME Hercules Cluster
Ref:	=1987AJ.....93..788D
by	DICKEY J.M. , KELLER D.T., PENNINGTON R., SALPETER E.E.
	Astron. J., 93, 788-804 (1987)
	A catalog of galaxies in Hercules from the Palomar sky survey and the Minnesota automated plate scanner.
o	Table V: <[DKP87] HHMMSS.ss+DDMMSS.s> N=667
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DKR2012]
[DKR2012]	(DALL'ORA+KINEMUCHI+RIPEPI+, 2012)
Write:	<<[DKR2012] V1>>
N:	1 (SIMBAD class: RRLyrae = RR Lyrae Variable)
Note:	WIRO 2.3 m telescope, Lowell Observatory 1.8 m Perkins telescope, and Loiano Observatory 1.5 m telescope observations of NAME UMA II Galaxy.
in source:	NAME UMa II Galaxy
Ref:	=2012ApJ...752...42D
by	DALL'ORA M. , KINEMUCHI K., RIPEPI V., RODGERS C.T., CLEMENTINI G., DI FABRIZIO L., SMITH H.A., MARCONI M., MUSELLA I., GRECO C., KUEHN C.A., CATELAN M., PRITZL B.J., BEERS T.C.
	Astrophys. J., 752, 42 (2012)
	Stellar archaeology in the Galactic halo with the ultra-faint dwarfs. VI. Ursa Major II.
o	Table 3: <[DKR2012] V1> N=1
=E=	Catalogue in electronic form as <J/ApJ/752/42/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DKR2014]
[DKR2014]	(Diaz+Koyama+Ryan-Weber+, 2014)
Write:	<<[DKR2014] JHHMMSS.ss+DDMMSS.s>>
N:	233+4
Object:	G (SIMBAD class: Galaxy)
Note:	Subaru Suprime-Cam observations of N=233+4 galaxies in two independant quasar lines of sight: SDSS J103027.01+052455.0 and SDSS J113717.73+354956.9 (Paper I, 2014MNRAS.442..946D). Keck-II DEIMOS spectroscopic follow-up, in Paper II (2015MNRAS.448.1240D).
Ref:	=2014MNRAS.442..946D
by	DIAZ C.G. , KOYAMA Y., RYAN-WEBER E.V., COOKE J., OUCHI M., SHIMASAKU K., NAKATA F.
	Mon. Not. R. Astron. Soc., 442, 946-978 (2014)
	Large-scale environment of z ~ 5.7 C IV absorption systems - I. Projected distribution of galaxies.
o	Tables E1-E6: <[DKR2014] JHHMMSS.ss+DDMMSS.s> N=233.
Ref:	=2015MNRAS.448.1240D
by	DIAZ C.G. , RYAN-WEBER E.V., COOKE J., KOYAMA Y., OUCHI M.
	Mon. Not. R. Astron. Soc., 448, 1240-1270 (2015)
	Large-scale environment of z ~ 5.7 Civ absorption systems -II. Spectroscopy of Lyman α emitters.
o	Table A1: <[DKR2014] JHHMMSS.ss+DDMMSS.s> (Nos J102951.56+052805.6, J103032.05+05:19:28.7, J102956.06+052128.6, J103026.91+053701.6) added.
=E=	Catalogue in electronic form as J/MNRAS/442/946
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DKS2007]
[DKS2007]	(Davis+Kumar+Sandell+, 2007)
Write:	<<[DKS2007] NN>> <<[DKS2007] DR21-IRSNN>> <<[DKS2007] W75N-IRSNN>> <<[DKS2007] L906E-IRSN>> <<[DKS2007] DR21WW>> <<[DKS2007] DR21WN>> <<[DKS2007] DR21(OH)WW>> <<[DKS2007] DR21(OH)WN>> <<[DKS2007] W75N-WN>> <<[DKS2007] A NN-N>> <<[DKS2007] a>>
N:	10+14+6+5+5+8+81+13
Object:	(IR) + H2 Knot + YSO (SIMBAD class: Infrared = Infra-Red Source)
Note:	UKIRT WFCAM near-IR images of DR 21-W 75 star-forming region.
in source:	DR 21
in source:	W 75
Ref:	=2007MNRAS.374...29D
by	DAVIS C.J. , KUMAR M.S.N., SANDELL G., FROEBRICH D., SMITH M.D., CURRIE M.J.
	Mon. Not. R. Astron. Soc., 374, 29-53 (2007)
	WFCAM, Spitzer/IRAC and SCUBA observations of the massive star-forming region DR21/W75 - I. The collimated molecular jets.
o	Table 1 col(1): <[DKS2007] NN> (Nos 1-37). Fig.2, Table 1, col(9): <[DKS2007] DR21-IRSNN> (Nos 1-10). Fig.3, Table 1, col(9): <[DKS2007] W75N-IRSNN> (Nos 1-14). Fig.6, Table 1, col(9): <[DKS2007] L906E-IRSN> (Nos 1-6). Table 2: <[DKS2007] DR21WW>, <[DKS2007] DR21WN>, N=5, <[DKS2007] DR21(OH)WW> N=5, <[DKS2007] W75NWN>, N=8. Table 3: <[DKS2007] A NN-N> N=81. Table 4, col(2): <[DKS2007] a> (Nos a-n, i missing). Table 2: <[CGC93] FIR NNa> (Nos 4-12, 5b) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DKV2003]
[DKV2003]	(Di Stefano+Kong+VanDalfsen+, 2003)
Write:	<<[DKV2003] XNNN>>
N:	122
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS observations of the Sombrero galaxy = M 104.
in source:	Sombrero galaxy = M 104 = NGC 4594
Ref:	=2003ApJ...599.1067D
by	DI STEFANO R. , KONG A.K.H., VANDALFSEN M.L., HARRIS W.E., MURRAY S.S., DELAIN K.M.
	Astrophys. J., 599, 1067-1081 (2003)
	X-ray point sources in the Sombrero galaxy: very soft sources, the globular cluster/low-mass X-ray binary connection, and an overview.
o	T.1: CXOU names for the objects have been created by truncating coordinates from Table 1.
o	Table 1: <[DKV2003] XNNN> (Nos X1-X122).
=E=	Catalogue in electronic form as J/ApJ/599/1067
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DKW2000]
[DKW2000]	(Dumke+Krause+Wielebinski, 2000)
Write:	<<[DKW2000] NGC 5907 SN>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=2 radio-sources (Nos S1-S2) in NGC 5907, identical to the 2 [HSE84] sources.
in source:	NGC 5907
Ref:	=2000A&A...355..512D
by	DUMKE M. , KRAUSE M., WIELEBINSKI R.
	Astron. Astrophys., 355, 512-524 (2000)
	The interstellar medium in the edge-on galaxy NGC 5907. Radio continuum emission and magnetic fields.
o	source 2234+28 not identified
o	Table 2: <[DKW2000] NGC 5907 SN> (Nos S1-S2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DKW2019]
[DKW2019]	(Delchambre+Krone-Martins+Wertz+, 2019)
Write:	<<[DKW2019] NN>>
N:	15
Object:	Poss. Grav. lens system (SIMBAD class: GravLensSystem_Candidate = Gravitational Lens System (lens+images) Candidate)
Note:	N=15 gravitational lens system candidates in Gaia DR2.
Ref:	=2019A&A...622A.165D
by	DELCHAMBRE L. , KRONE-MARTINS A., WERTZ O., DUCOURANT C., GALLUCCIO L., KLUTER J., MIGNARD F., TEIXEIRA R., DJORGOVSKI S.G., STERN D., GRAHAM M.J., SURDEJ J., BASTIAN U., WAMBSGANSS J., LE CAMPION J.-F., SLEZAK E.
	Astron. Astrophys., 622A, 165-165 (2019)
	Gaia GraL: Gaia DR2 Gravitational Lens Systems. III. A systematic blind search for new lensed systems.
o	Fig. 4, Table 3: <[DKW2019] NN> N=15 among (Nos 4-30).
o	J2145+6345 is Gaia DR2 2216740923364878464 in SIMBAD.
=E=	Catalogue in electronic form as <J/A+A/622/A165/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DKZ2005]
[DKZ2005]	(Dieball+ Knidge+Zurek+, 2005)
Write:	<<[DKZ2005] NNN>>
N:	521
Object:	(Far UV) (SIMBAD class: UV = UV-emission Source)
Note:	New analysis of FUV observations of NGC 2808 obtained with the HST.
in source:	NGC 2808
Ref:	=2005ApJ...625..156D
by	DIEBALL A. , KNIGGE C., ZUREK D.R., SHARA M.M., LONG K.S.
	Astrophys. J., 625, 156-166 (2005)
	Far-ultraviolet observations of the globular cluster NGC 2808 revisited: blue stragglers, white dwarfs, and cataclysmic variables.
o	Table 1: <[DKZ2005] NNN> (Nos 1-521).
=E=	Catalogue in electronic form as J/ApJ/625/156
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DKZ2007]
[DKZ2007]	(Dieball+ Knidge+Zurek+, 2007)
Write:	<<[DKZ2007] NNNN>>
N:	2731
Object:	UV (SIMBAD class: UV = UV-emission Source)
Note:	HST ACS images of M 15.
in source:	M 15 = NGC 7078
Ref:	=2007ApJ...670..379D
by	DIEBALL A. , KNIGGE C., ZUREK D.R., SHARA M.M., LONG K.S., CHARLES P.A., HANNIKAINEN D.
	Astrophys. J., 670, 379-399 (2007)
	Unveiling the core of the globular cluster M15 in the ultraviolet.
o	(Erratum) erratum vol. 708, p. 1772 (2010)
o	Table 2: <[DKZ2007] NNNN> (Nos 1-2731).
=E=	Catalogue in electronic form as J/ApJ/670/379
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DL
DL	(Dust Lane)
*****	Avoid the usage of DL, prefer [CGC77]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DLA2012]
[DLA2012]	(Danielson+Lehmer+Alexander+, 2012)
Write:	<<[DLA2012] DDD.ddddddd+DD.ddddddd>>
N:	393
Object:	Early-type G (SIMBAD class: Galaxy)
Note:	N=393 early-type galaxies in the Chandra Deep Field-North and -South.
in source:	NAME CDFS
in source:	NAME CDFN
Ref:	=2012MNRAS.422..494D
by	DANIELSON A.L.R. , LEHMER B.D., ALEXANDER D.M., BRANDT W.N., LUO B., MILLER N., XUE Y.Q., STOTT J.P.
	Mon. Not. R. Astron. Soc., 422, 494-509 (2012)
	The cosmic history of hot gas cooling and radio active galactic nucleus activity in massive early-type galaxies.
o	Table 1: <[DLA2012] DDD.ddddddd+DD.ddddddd> N=393.
=E=	Catalogue in electronic form as J/MNRAS/422/494
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLB87]
[DLB87]	(Dressler+Lynden-Bell+Burstein+, 1987)
Write:	<<[DLB87] ANN>>
N:	20+8+16+11+14+28
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=20 galaxies in Virgo cluster, (Nos V1-V20). N=8 galaxies in Fornax cluster, (Nos F1-F8). N=16 galaxies in Perseus cluster, (Nos P1-P16). N=11 galaxies in DRCG 2345-28, (Nos D1-D11). N=14 galaxies in ACO 2199, (Nos A1-A14). N=28 galaxies in Coma cluster, (Nos C1-C28).
in source:	NAME Virgo Cluster
in source:	NAME Fornax Cluster
in source:	NAME Perseus Cluster
in source:	DRCG 2345-28
in source:	ACO 2199
in source:	Coma Cluster = ACO 1656
Ref:	=1987ApJ...313...42D
by	DRESSLER A. , LYNDEN-BELL D., BURSTEIN D., DAVIES R.L., FABER S.M., TERLEVICH R.J., WEGNER G.
	Astrophys. J., 313, 42-58 (1987)
	Spectroscopy and photometry of elliptical galaxies. I. A new distance estimator.
o	Table 2, col(3): sample numbering 'NNN' in authors complete survey not used in SIMBAD.
o	Table 2: <[DLB87] VNN> (Nos V1-V20), <[DLB87] FN> (Nos F1-F8), <[DLB87] PNN> (Nos P1-P16), <[DLB87] DNN> (Nos D1-D11), <[DLB87] ANN> (Nos A1-A14), <[DLB87] CNN> (Nos C1-C28).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLC2022]
[DLC2022]	(Dong+Liu+Cuello+, 2022)
Write:	<<[DLC2022] A>>
N:	4
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA 224GHz (1.3mm) and JVLA 33 GHz (9mm) observations of N=4 point-like sources in the field of the binary protostar Z CMa.
Ref:	=2022NatAs...6..331D
by	DONG R. , LIU H.B., CUELLO N., PINTE C., ABRAHAM P., VOROBYOV E., HASHIMOTO J., KOSPAL A., CHIANG E., TAKAMI M., CHEN L., DUNHAM M., FUKAGAWA M., GREEN J., HASEGAWA Y., HENNING T., PAVLYUCHENKOV Y., PYO T.-S., TAMURA M.
	NatAs, 6, 331-338 (2022)
	A likely flyby of binary protostar Z CMa caught in action.
o	Fig. 1, Ext. Data Fig. 3: <[DLC2022] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLC97]
[DLC97]	(Deltorn+Le Fevre+Crampton+, 1997)
Write:	<<[DLC97] NNNN>>
N:	11
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Table 1: N=11 galaxies from the authors' photometric catalog of a cluster of galaxies around 3CR 184.
in source:	NAME 3C 184 Cluster
Ref:	=1997ApJ...483L..21D
by	DELTORN J.-M. , LE FEVRE O., CRAMPTON D., DICKINSON M.
	Astrophys. J., 483, 21-24 (1997)
	A massive cluster of galaxies at z = 0.996.
o	Table 1: <[DLC97] NNNN> N=11 among N>1168
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLF2005]
[DLF2005]	(Durret+Lima Neto+Forman, 2005)
Write:	<<[DLF2005] NN>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of ACO 85. N=17 point sources.
in source:	ACO 85
Ref:	=2005A&A...432..809D
by	DURRET F. , LIMA NETO G.B., FORMAN W.
	Astron. Astrophys., 432, 809-821 (2005)
	An XMM-Newton view of the cluster of galaxies Abell 85.
o	Table 1: <[DLF2005] NN> (Nos 1-17).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLF2014]
[DLF2014]	(David+Lim+Forman+, 2014) (Not yet in Simbad)
Write:	<<[DLF2014] NGC 5044 NN>>
N:	26
Object:	Poss. MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	ALMA observations of N=24+2 molecular cloud candidates in NGC 5044. See also [TAG2018] for NGC 5846 and NGC 4636.
in source:	NAME NGC 5044 GROUP:NGC 5044 = NGC 5044
Ref:	=2014ApJ...792...94D
by	DAVID L.P. , LIM J., FORMAN W., VRTILEK J., COMBES F., SALOME P., EDGE A., HAMER S., JONES C., SUN M., O'SULLIVAN E., GASTALDELLO F., BARDELLI S., TEMI P., SCHMITT H., OHYAMA Y., MATHEWS W., BRIGHENTI F., GIACINTUCCI S., TRUNG D.-V.
	Astrophys. J., 792, 94 (2014)
	Molecular gas in the X-ray bright group NGC 5044 as revealed by ALMA.
o	Fig. 2, Table 1: <[DLF2014] NGC 5044 NN> (Nos 1-24).
Ref:	=2018ApJ...858...17T
by	TEMI P. , AMBLARD A., GITTI M., BRIGHENTI F., GASPARI M., MATHEWS W.G., DAVID L.
	Astrophys. J., 858, 17-17 (2018)
	ALMA observations of molecular clouds in three group-centered elliptical galaxies: NGC 5846, NGC 4636, and NGC 5044.
o	Table 3: <[TAG2018] NGC NNNN NN> N=3+2. Fig. 1, Table 3: <[DLF2014] NGC 5044 NN> (Nos 25-26) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLG2010]
[DLG2010]	(D'Orazi+Lucatello+Gratton+, 2010)
Write:	<<[DLG2010] NNN>>
N:	114
Object:	* (SIMBAD class: Star)
Note:	Use of ESO archival FLAMES-Giraffe observations of the metal-rich globular cluster 47 Tuc.
in source:	NGC 104 = 47 Tuc
Ref:	=2010ApJ...713L...1D
by	D'ORAZI V. , LUCATELLO S., GRATTON R., BRAGAGLIA A., CARRETTA E., SHEN Z., ZAGGIA S.
	Astrophys. J., 713L, 1-5 (2010)
	Lithium and proton-capture elements in globular cluster dwarfs: the case of 47 Tuc.
o	Table 1: <[DLG2010] NNN> (Nos 1-114).
=E=	Catalogue in electronic form as <J/ApJ/713/L1/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DLIRIM
DLIRIM	(Diffraction Limited IR Imaging)
*****	Avoid the usage of DLIRIM, prefer [WKG96]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DLK2001]
[DLK2001]	(Dinh-V-Trung+Lo+Kim+, 2001)
Write:	<<[DLK2001] IRAS FHHMMm+DDMM W>>
N:	12
Object:	G in Pair (SIMBAD class: GinPair = Galaxy in Pair of Galaxies)
Note:	6X2 IRAS FSC are ULIRGs pairs.
in source:	IRAS F10485-1447
in source:	IRAS F11180+1623
in source:	IRAS F12359-0725
in source:	IRAS F14394+5332
in source:	IRAS F17028+5817
in source:	IRAS F23327+2913
Ref:	=2001ApJ...556..141D
by	DINH-V-TRUNG , LO K.Y., KIM D.-C., GAO Y., GRUENDL R.A.
	Astrophys. J., 556, 141-149 (2001)
	Nature of widely separated ultraluminous infrared galaxies.
o	Table 3: <[DLK2001] IRAS FHHMMm+DDMM W> N=6x2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLK2008]
[DLK2008]	(Deharveng+Lefloch+Kurtz+, 2008)
Write:	<<[DLK2008] NNN>> <<[DLK2008] CN>>
N:	925+5
Object:	* + Condensation (SIMBAD class: Star)
Note:	CFHT NIR and IRAM 30m CO/CS observations of Sh 2-212.
in source:	SH 2-212
Ref:	=2008A&A...482..585D
by	DEHARVENG L. , LEFLOCH B., KURTZ S., NADEAU D., POMARES M., CAPLAN J., ZAVAGNO A.
	Astron. Astrophys., 482, 585-596 (2008)
	Triggered massive-star formation on the borders of Galactic HII regions. IV. Star formation at the periphery of Sh2-212.
o	Table 3: <[DLK2008] NNN> (Nos 1-925). Fig.8, Table 5: <[DLK2008] CN> (Nos C1-C5).
=E=	Catalogue in electronic form as <J/A+A/482/585/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLK2010]
[DLK2010]	(Dieball+Long+Knigge+, 2010)
Write:	<<[DLK2010] NNNNN>>
N:	3168
Object:	(FUV) (SIMBAD class: UV = UV-emission Source)
Note:	HST ACS UV observations of the core region of M80.
in source:	NGC 6093 = M 80
Ref:	=2010ApJ...710..332D
by	DIEBALL A. , LONG K.S., KNIGGE C., THOMSON G.S., ZUREK D.R.
	Astrophys. J., 710, 332-345 (2010)
	A far-ultraviolet survey of M80: X-ray source counterparts, strange blue stragglers, and the recovery of nova T Sco.
o	Table 1: <[DLK2010] NNNNN> N=3168 among (Nos 1-10007).
=E=	Catalogue in electronic form as J/ApJ/710/332
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLK2013]
[DLK2013]	(Diener+Lilly+Knobel+, 2013)
Write:	<<[DLK2013] NN>>
N:	42
Object:	Poss. Group of G (SIMBAD class: GroupG_Candidate = Group of Galaxies Candidate)
Note:	N=42 candidate groups lying between 1.8<z<3.0 from a sample of 3502 galaxies with spectroscopic redshifts in the zCOSMOS-deep redshift survey.
Ref:	=2013ApJ...765..109D
by	DIENER C. , LILLY S.J., KNOBEL C., ZAMORANI G., LEMSON G., KAMPCZYK P., SCOVILLE N., CAROLLO C.M., CONTINI T., KNEIB J.-P., LE FEVRE O., MAINIERI V., RENZINI A., SCODEGGIO M., BARDELLI S., BOLZONELLA M., BONGIORNO A., CAPUTI K., CUCCIATI O., DE LA TORRE S., DE RAVEL L., FRANZETTI P., GARILLI B., IOVINO A., KOVAC K., LAMAREILLE F., LE BORGNE J.-F., LE BRUN V., MAIER C., MIGNOLI M., PELLO R., PENG Y., PEREZ MONTERO E., PRESOTTO V., SILVERMAN J., TANAKA M., TASCA L., TRESSE L., VERGANI D., ZUCCA E., BORDOLOI R., CAPPI A., CIMATTI A., COPPA G., KOEKEMOER A.M., LOPEZ-SANJUAN C., McCRACKEN H.J., MORESCO M., NAIR P., POZZETTI L., WELIKALA N.
	Astrophys. J., 765, 109 (2013)
	Proto-groups at 1.8 < z < 3 in the zCOSMOS-deep sample.
o	Table 1: <[DLK2013] NN> (Nos 1-42).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLL2002]
[DLL2002]	(Dannerbauer+Lehnert+Lutz+, 2002)= (MM)
Write:	<<[DLL2002] MM JHHMMSS+DDMM.m>>
N:	18
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Search for millimeter galaxies in the NTT (New Technology Telescope) Deep Field. See also [DLL2004], [EBI2003].
Ref:	=2002ApJ...573..473D
by	DANNERBAUER H. , LEHNERT M.D., LUTZ D., TACCONI L., BERTOLDI F., CARILLI C., GENZEL R., MENTEN K.
	Astrophys. J., 573, 473-484 (2002)
	Properties of millimeter galaxies: constraints from K-band blank fields.
o	p. 478 : IRAS 15250+0309 is a misprint for IRAS 15250+3609 ?
o	Table 1: <[DLL2002] MM JHHMMSS+DDMM.m> N=3.
Ref:	=2004ApJ...606..664D
by	DANNERBAUER H. , LEHNERT M.D., LUTZ D., TACCONI L., BERTOLDI F., CARILLI C., GENZEL R., MENTEN K.M.
	Astrophys. J., 606, 664-682 (2004)
	The faint counterparts of MAMBO millimeter sources near the New Technology Telescope Deep Field.
o	Introd. : SMM 02399-0314 is a misprint for SMM J02399-0134, Parag. 4 : LE 850.12 = [SFD2002] LHE 12
o	Table 1, col(1): <[DLL2002] MM JHHMMSS+DDMM.m> N=15 added. Table 1, col(2): <[EBI2003] NTT-MM NN> N=12 added among (Nos 7-42). Table 1, col(6,7): <DLL2004] JHHMMSS.ss+DDMMSS.s> N=23. Table 2: <[DLL2004] MAMBO NTT -MM NNaN> N=82.
=E=	Catalogue in electronic form as J/ApJ/606/664
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLL2004]
[DLL2004]	(Dannerbauer+Lehnert+Lutz+, 2004)= MAMBO
Write:	<<[DLL2004] JHHMMSS.ss+DDMMSS.s>> <<[DLL2004] MAMBO NTT-MM NNaN>>
N:	23+82
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLA, IRAM et ESO observations. Search for counterparts to the 18 [EBI2003] mm sources in the NTT (New Technology Telescope) Deep Field (designated [EBI2003] NTT-MM NN, synonymous with MAMBO NTT-MM NN in SIMBAD). N=23 radio-sources are associated with the mm sources. N=82 optical-NIR objects close to the mm sources. Some of these objects are suggested as counterpart to mm sources by the authors. See also [DLL2002].
Ref:	=2004ApJ...606..664D
by	DANNERBAUER H. , LEHNERT M.D., LUTZ D., TACCONI L., BERTOLDI F., CARILLI C., GENZEL R., MENTEN K.M.
	Astrophys. J., 606, 664-682 (2004)
	The faint counterparts of MAMBO millimeter sources near the New Technology Telescope Deep Field.
o	Introd. : SMM 02399-0314 is a misprint for SMM J02399-0134, Parag. 4 : LE 850.12 = [SFD2002] LHE 12
o	Table 1, col(1): <[DLL2002] MM JHHMMSS+DDMM.m> N=15 added. Table 1, col(2): <[EBI2003] NTT-MM NN> N=12 added among (Nos 7-42). Table 1, col(6,7): <DLL2004] JHHMMSS.ss+DDMMSS.s> N=23. Table 2: <[DLL2004] MAMBO NTT -MM NNaN> N=82.
=E=	Catalogue in electronic form as J/ApJ/606/664
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLL2015]
[DLL2015]	(De Los Reyes+Ly+Lee+, 2015)= ([DLL2015a])
Write:	<<[DLL2015] SXDSW-NNNNN>>
N:	299
Object:	G (SIMBAD class: Galaxy)
Note:	KPNO/CTIO 4-m telescopes NEWFIRM and Magellan 6.5-m Baade telescope FourStar NIR narrowband photometry. Magellan-I telescope IMACS spectroscopy of N=299 Hα-selected galaxies at z∼0.8 from the NEWFIRM NewHα survey.
in source:	NAME SXDF
Ref:	=2015AJ....149...79D
by	DE LOS REYES M.A. , LY C., LEE J.C., SALIM S., PEEPLES M.S., MOMCHEVA I., FEDDERSEN J., DALE D.A., OUCHI M., ONO Y., FINN R.
	Astron. J., 149, 79 (2015)
	The relationship between stellar mass, gas metallicity, and star formation rate for Hα-selected galaxies at z ~~ 0.8 from the NewHα survey.
o	Tables 1-5: <[DLL2015] SXDSW-NNNNN> N=299.
=E=	Catalogue in electronic form as J/AJ/149/79
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLL2015a]
[DLL2015a]	(De Los Reyes+Ly+Lee+, 2015)
*****	Avoid the usage of [DLL2015a], prefer [DLL2015]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLL2015b]
[DLL2015b]	(Diener+Lilly+Ledoux+, 2015)
Write:	<<[DLL2015b] protocluster>> <<[DLL2015b] NNNNNNN>>
N:	11+1
Object:	Protocluster + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT FORS2 observations of N=11 galaxy members of a protocluster at z=2.45.
Ref:	=2015ApJ...802...31D
by	DIENER C. , LILLY S.J., LEDOUX C., ZAMORANI G., BOLZONELLA M., MURPHY D.N.A., CAPAK P., ILBERT O., McCRACKEN H.
	Astrophys. J., 802, 31 (2015)
	A protocluster at z = 2.45.
o	Table 1: <[DLL2015b] NNNNNNN> N=11 among (Nos 409614-1034036), <[DLL2015b] protocluster> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLL2020]
[DLL2020]	(Dutta+Lee+Liu+, 2020)
Write:	<<[DLL2020] GLLL.ll-BB.bb A>> <<[DLL2020] GLLL.ll-BB.bbW A>> <<[DLL2020] GLLL.ll-BB.bbWN A>> <<[DLL2020] GLLL.ll-BB.bbM A>> <<[DLL2020] GLLL.ll-BB.bbMN A>> <<[DLL2020] G208.89-20.04Walma>>
N:	70
Object:	Dense Core (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	ALMA band 6 (1.3mm) observations of N=70 young dense cores in the Orion Complex, as part of the ALMA survey of Orion Planck Galactic Cold Clumps (ALMASOP).
in source:	NAME Ori Complex
Ref:	=2020ApJS..251...20D
by	DUTTA S. , LEE C.-F., LIU T., HIRANO N., LIU S.-Y., TATEMATSU K., KIM K.-T., SHANG H., SAHU D., KIM G., MORAGHAN A., JHAN K.-S., HSU S.-Y., EVANS N.J., JOHNSTONE D., WARD-THOMPSON D., KUAN Y.-J., LEE C.W., LEE J.-E., TRAFICANTE A., JUVELA M., VASTEL C., ZHANG Q., SANHUEZA P., SOAM A., KWON W., BRONFMAN L., EDEN D., GOLDSMITH P.F., HE J., WU Y., PELKONEN V.-M., QIN S.-L., LI S., LI D.
	Astrophys. J., Suppl. Ser., 251, 20-20 (2020)
	ALMA survey of Orion Planck Galactic Cold Clumps (ALMASOP). II. Survey overview: a first look at 1.3 mm continuum maps and molecular outflows.
o	Table 5: <[DLL2020] GLLL.ll-BB.bb A>, <[DLL2020] GLLL.ll-BB.bbW A>, <[DLL2020] GLLL.ll-BB.bbWN A>, <[DLL2020] GLLL.ll-BB.bbMN A>, <[DLL2020] G208.89-20.04Walma>, N=70.
=E=	Catalogue in electronic form as <J/ApJS/251/20/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [DLL99]
[DLL99]	(Diamond+Lonsdale+Lonsdale+, 1999) (Not yet in Simbad)
Write:	<<[DLL99] WN>>
N:	5
Object:	OH Maser (SIMBAD class: Maser)
Note:	N=5 regions of OH Maser cluster in Zw III 35. See also [TMG97]
in source:	ZW III 35
Ref:	=1999ApJ...511..178D
by	DIAMOND P.J. , LONSDALE C.J., LONSDALE C.J., SMITH H.E.
	Astrophys. J., 511, 178-184 (1999)
	Global VLBI observations of the compact OH megamaser emission from III Zw 35 and IRAS 17208-0014.
o	Fig.1: <[DLL99] WN> (Nos S11-S2. N2-N3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLM2003]
[DLM2003]	(De grijs+Lee+Mora Herrera+, 2003)= [DLM2003a]
Write:	<<[DLM2003] Mice NN>> <<[DLM2003] Tadpole NN>>
N:	45+38
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST observations are used to explore and deduce the star and star cluster formation histories in The Mice and the Tadpole interacting galaxies.
in source:	Mice = NGC 4676
in source:	Tadpole Galaxy = VV 29
Ref:	=2003NewA....8..155D
by	DE GRIJS R. , LEE J.T., MORA HERRERA M.C., FRITZE-v.ALVENSLEBEN U., ANDERS P.
	New Astronomy, 8, 155-None (2003)
	Stellar populations and star cluster formation in interacting galaxies with the Advanced Camera for Surveys.
o	Table 1: <[DLM2003] Mice NN> (Nos 1-45). Table 2: <[DLM2003] Tadpole NN> (Nos 1-38).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLM2003a]
[DLM2003a]	(De grijs+Lee+Mora Herrera+, 2003)
*****	Avoid the usage of [DLM2003a], prefer [DLM2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLM2003b]
[DLM2003b]	(Dodson+Lewis+McConnell+, 2003)
Write:	<<[DLM2003b] FR-II>> <<[DLM2003b] JHHMMSS.s+DDMMSS>>
N:	1+3
Object:	G + (X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra X-ray observations of the Vela pulsar. N=1 bright background galaxy 'FR-II', and N=3 point sources in the field of the pulsar.
Ref:	=2003MNRAS.343..116D
by	DODSON R. , LEWIS D., McCONNELL D., DESHPANDE A.A.
	Mon. Not. R. Astron. Soc., 343, 116-124 (2003)
	The radio nebula surrounding the Vela pulsar.
o	Text: <[DLM2003b] FR-II> N=1, <[DLM2003b] JHHMMSS.s+DDMMSS> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLM2005]
[DLM2005]	(Dennefeld+Lagache+Mei+, 2005)
Write:	<<[DLM2005] FN1 NNNA>>
N:	9
Object:	? (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Search for possible optical ID of FIRBACK sources. See also [CSI2002], [PDL2003].
Ref:	=2005A&A...440....5D
by	DENNEFELD M. , LAGACHE G., MEI S., CILIEGI P., DOLE H., MANN R.G., TAYLOR E.L., VACCARI M.
	Astron. Astrophys., 440, 5-22 (2005)
	FIRBACK. IV. Towards the nature of the 170 µm source population.
o	sources FN 1-126 and 295 not identified.
o	Tables 2, 3: <[DLM2005] FN1 NNNA> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLM2010]
[DLM2010]	(Dzib+Loinard+Mioduszewski+, 2010)
Write:	<<[DLM2010] EC 95a>>
N:	2
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	VLBA 3.6cm observations of the binary system [EC92] 95.
in source:	[EC92] 95
Ref:	=2010ApJ...718..610D
by	DZIB S. , LOINARD L., MIODUSZEWSKI A.J., BODEN A.F., RODRIGUEZ L.F., TORRES R.M.
	Astrophys. J., 718, 610-619 (2010)
	VLBA determination of the distance to nearby star-forming regions. IV. A preliminary distance to the Proto-Herbig AeBe star EC 95 in the Serpens core.
o	<[DLM2010] EC 95a> (Nos EC 95a-EC 95b).
o	The 4 calibrators are not in SIMBAD.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLM2016]
[DLM2016]	(Dalessandro+Lapenna+Mucciarelli+, 2016)
Write:	<<[DLM2016] NN>>
N:	5
Object:	Giant * (SIMBAD class: Star)
Note:	HST WFC3 (UVIS) photometry and VLT FLAMES UVES spectroscopy of N=5 giant stars in the massive globular cluster NGC 121.
in source:	NGC 121
Ref:	=2016ApJ...829...77D
by	DALESSANDRO E. , LAPENNA E., MUCCIARELLI A., ORIGLIA L., FERRARO F.R., LANZONI B.
	Astrophys. J., 829, 77-77 (2016)
	Multiple populations in the old and massive Small Magellanic Cloud globular cluster NGC 121.
o	Tables 1-3: <[DLM2016] NN> N=5 among (Nos 9-35).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLP96]
[DLP96]	(Digel+Lyder+Philbrick+, 1996)
Write:	<<[DLP96] NN>>
N:	59
Object:	Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
in source:	NAME Perseus Arm
Ref:	=1996ApJ...458..561D
by	DIGEL S.W. , LYDER D.A., PHILBRICK A.J., PUCHE D., THADDEUS P.
	Astrophys. J., 458, 561-575 (1996)
	A large-scale CO survey toward W3, W4, and W5.
o	p. 564: LBN 656 = LBN 135.10+0.09, LBN 657 = LBN 135.13+0.01. Fig. 6: Lo 1 = [L89b] 132.157-00.725, Lo 2 = [L89b] 136.913+1.033
o	Table 3: <[DLP96] NN> (Nos 1-59). Fig. 6: <NAME Lo N> (Nos 1-2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLR2016]
[DLR2016]	(Dey+Lee+Reddy+, 2016)
Write:	<<[DLR2016] PC 217.96+32.3>> <<[DLR2016] LAENNNNN>>
N:	1+165
Object:	Protocluster + Poss. LAE (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Mayall MOSAIC1.1 imaging and Keck II DEIMOS spectroscopy of objects in the field of a protocluster at z=3786. N=165 candidate Lymanα emitting galaxies (LAEs).
Ref:	=2016ApJ...823...11D
by	DEY A. , LEE K.-S., REDDY N., COOPER M., INAMI H., HONG S., GONZALEZ A.H., JANNUZI B.T.
	Astrophys. J., 823, 11-11 (2016)
	Spectroscopic confirmation of a protocluster at z~3.786.
o	<[DLR2016] PC 217.96+32.3> N=1. Tables 3-4: <[DLR2016] LAENNNNN> N=165 among (Nos 1257-56824).
=E=	Catalogue in electronic form as <J/ApJ/823/11/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DLS
DLS	(Deep Lens Survey)
Write:	<<DLS JHHMMSS.ss+DDMMSS.s>>
N:	about 10000000
Object:	G + * (SIMBAD class: Galaxy)
Note:	Deep BVRz imaging of 20 sq.deg. (5 widely separated 2x2 deg fields). Main purpose is gravitational lensing galaxies and clusters. See also DLSCL for clusters. http://dls.physics.ucdavis.edu
Auth.:	WITTMAN D.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: DLS
DLS	(Deep Lens Survey)
*****	Avoid the usage of DLS, prefer [KD2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DLS2013]
[DLS2013]	(de Hoon+Lamer+Schwope+, 2013)
Write:	<<[DLS2013] N>> <<[DLS2013] JHHMMSS.s+DDMMSS.s>> <<[DLS2013] N A>>
N:	9+231+66
Object:	(X) + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT FORS2 observations of N=231 galaxies in N=9 extended X-ray sources in a deep XMM-Newton field, including N=66 cluster members.
Ref:	=2013A&A...551A...8D
by	DE HOON A. , LAMER G., SCHWOPE A., MUEHLEGGER M., FASSBENDER R., BOEHRINGER H., LERCHSTER M., NASTASI A., SUHADA R., VERDUGO M., DIETRICH J.P., BRIMIOULLE F., ROSATI P., PIERINI D., SANTOS J.S., QUINTANA H., RABITZ A., TAKEY A.
	Astron. Astrophys., 551A, 8-8 (2013)
	Distant galaxy clusters in a deep XMM-Newton field within the CFTHLS D4.
o	Fig. 1, Tables 3+4+7: <[DLS2013] N> (Nos 1-9). Table 5: <[DLS2013] JHHMMSS.s+DDMMSS.s> N=231. Table 6: <[DLS2013] N A> N=66.
=E=	Catalogue in electronic form as J/A+A/551/A8
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLS93]
[DLS93]	(David+Le Squeren+Sivagnanam+, 1993)= ([DLS93a])
Write:	<<[DLS93] HHMMm+DDMMa>>
N:	131
Object:	Maser (SIMBAD class: Maser)
Note:	Nancay Radio Telescope 1667MHz observations of N=131 masers towards IRAS sources. See also [DLS93b].
Ref:	=1993A&AS...98..245D
by	DAVID P. , LE SQUEREN A.M., SIVAGNANAM P., BRAZ M.A.
	Astron. Astrophys., Suppl. Ser., 98, 245-260 (1993)
	An OH mainline maser survey of IRAS circumstellar envelope sources.
o	In table 2 IRAS 08005+2356 is a misprint for IRAS 08005-2356.
o	Tables 1-2: <[DLS93] HHMMm+DDMMa> N=89+42.
Details on Acronym: [DLS93a]
[DLS93a]	(David+Le Squeren+Sivagnanam+, 1993)
*****	Avoid the usage of [DLS93a], prefer [DLS93]
Details on Acronym: [DLS93b]
[DLS93b]	(David+Le Squeren+Sivagnanam, 1993)
Write:	<<[DLS93b] HHMMm+DDMMa>>
N:	141
Object:	Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	Nancay Radio Telescope 1612MHZ observations of N=141 masers towards IRAS sources. See also [DLS93].
Ref:	=1993A&A...277..453D
by	DAVID P. , LE SQUEREN A.M., SIVAGNANAM P.
	Astron. Astrophys., 277, 453-474 (1993)
	An OH satellite line maser survey of cool IRAS sources and circumstellar envelope evolution.
o	Table1, line 4, read IRAS 08005-2356 instead of 08005+2356.
o	Table 1: <[DLS93b] HHMMm+DDMMa> N=141.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DLSCL
DLSCL	(Deep Lens Survey, ClG)
Write:	<<DLSCL JHHMM.m+DDMM>>
N:	about 200
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	Deep BVRz imaging of 20 sq.deg. (5 widely separated 2x2 deg fields). Main purpose is gravitational lensing galaxies and clusters. see also DLS G or Stars. http://dls.physics.ucdavis.edu. 2005ApJ...635L.125G: 1st ref. with a DLSCL cluster.
Ref:	=2005ApJ...635L.125G
by	GELLER M.J. , DELL'ANTONIO I.P., KURTZ M.J., RAMELLA M., FABRICANT D.G., CALDWELL N., TYSON J.A., WITTMAN D.
	Astrophys. J., 635, 125-128 (2005)
	SHELS: the Hectospec Lensing Survey.
o	<DLSCL JHHMM.m+DDMM> N=1. <[GDK2005] JHHMMSS+DDMMSS> N=3.
Ref:	=2006ApJ...643..128W
by	WITTMAN D. , DELL'ANTONIO I.P., HUGHES J.P., MARGONINER V.E., TYSON J.A., COHEN J.G., NORMAN D.
	Astrophys. J., 643, 128-143 (2006)
	First results on shear-selected clusters from the Deep Lens Survey: optical imaging, spectroscopy, and X-ray follow-up.
o	Tables 1, 2: numbering N (Nos 1-8) is not used in SIMBAD, use DLSCL designation.
o	Table 2: <DLSCL JHHMM.m+DDMM> N=7 added. Fig.8: <[WDH2006] DLSCL J0920.1+3029 A> (Nos A-D). Fig.9: <[WDH2006] DLSCL J0522.2-4820 A> (Nos A-D).
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: DLT
DLT	(DLT40 Survey)
Write:	<<DLT YYaa>>
Object:	Transient (SIMBAD class: Transient = Transient Event)
Note:	CTIO PROMPT 0.4m telescope observations of transients, as part of the D<40Mpc (DLT40) survey. For more information, visit: http://dark.physics.ucdavis.edu/dlt40/DLT40 Only the first references citing DLT transients are listed here.
Ref:	=2016ATel.9782....1T
by	TARTAGLIA L. , SAND D., VALENTI S.
	ATel, 9782, 1 (2016)
	The discovery of DLT15am/AT 2016ija.
Ref:	=2017ATel10706....1V
by	VALENTI S. , TARTAGLIA L., SAND D., WYATT S., BOSTROEM K.A., REICHART D.E., HAISLIP J.B., KOUPRIANOV V.
	The Astronomer's Telegram, 10706, 1 (2017)
	The discovery of DLT17cq/AT 2017gmr with PROMPT.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DLT2009]
[DLT2009]	(De Ravel+Le Fevre+Tresse+, 2009)
Write:	<<[DLT2009] NN>> <<[DLT2009] pHHNNNNNNN>>
N:	36+3
Object:	Pair of G + G in Pair (SIMBAD class: PairG = Pair of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=36 pairs of galaxies from the VIMOS VLT Deep Survey (see also VVDS).
Ref:	=2009A&A...498..379D
by	DE RAVEL L. , LE FEVRE O., TRESSE L., BOTTINI D., GARILLI B., LE BRUN V., MACCAGNI D., SCARAMELLA R., SCODEGGIO M., VETTOLANI G., ZANICHELLI A., ADAMI C., ARNOUTS S., BARDELLI S., BOLZONELLA M., CAPPI A., CHARLOT S., CILIEGI P., CONTINI T., FOUCAUD S., FRANZETTI P., GAVIGNAUD I., GUZZO L., ILBERT O., IOVINO A., LAMAREILLE F., McCRACKEN H.J., MARANO B., MARINONI C., MAZURE A., MENEUX B., MERIGHI R., PALTANI S., PELLO R., POLLO A., POZZETTI L., RADOVICH M., VERGANI D., ZAMORANI G., ZUCCA E., BONDI M., BONGIORNO A., BRINCHMANN J., CUCCIATI O., DE LA TORRE S., GREGORINI L., MEMEO P., PEREZ-MONTERO E., MELLIER Y., MERLUZZI P., TEMPORIN S.
	Astron. Astrophys., 498, 379-397 (2009)
	The VIMOS VLT Deep Survey. Evolution of the major merger rate since z ~ 1 from spectroscopically confirmed galaxy pairs.
o	Table 2: <[DLT2009] NN> (Nos 1-36), <[DLT2009] pHHNNNNNNN> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLW2014]
[DLW2014]	(Dong+Li+Wang+, 2014)
Write:	<<[DLW2014] M31 A>>
N:	5
Object:	Dust Clump (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	Identification of N=5 dusty clumps in the central 200pc of M31. Use of archival HST WFC3 and ACS images and Swift UVOT data.
in source:	M 31 = NGC 224
Ref:	=2014ApJ...785..136D
by	DONG H. , LI Z., WANG Q.D., LAUER T.R., OLSEN K., SAHA A., DALCANTON J., GORDON K., FOUESNEAU M., BELL E., BIANCHI L.
	Astrophys. J., 785, 136 (2014)
	The panchromatic Hubble Andromeda treasury. VII. The steep mid-ultraviolet to near-infrared extinction curve in the central 200 pc of the M31 bulge.
o	Table 2: <[DLW2014] M31 A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLW84]
[DLW84]	(Dent+Little+White, 1984)
Write:	<<[DLW84] G35.2W>> <<[DLW84] G35.2WN>> <<[DLW84] G35.2W(UN)>>
N:	2+3+2
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=2 radio-sources North and South in the molecular cloud G35.2-0.74, identified as HII regions. The 'G35.2N' source has 3 components N1 to N3. The 'G35.2S' source contains 2 unresolved sources U1 and U2.
in source:	GAL 035.2-00.74
Ref:	=1984MNRAS.210..173D
by	DENT W.R.F. , LITTLE L.T., WHITE G.J.
	Mon. Not. R. Astron. Soc., 210, 173-181 (1984)
	Compact HII regions in the molecular cloud G 35.2-0.74.
o	Table 1: <[DLW84] G35.2W> (Nos G35.2N, G35.2S), <[DLW84] G35.2WN> (Nos G35.2N1, N2), <[DLW84] G35.2W(UN)> (Nos G35.2S(U1), (U2)).
Ref:	=1987MNRAS.229..679B
by	BREBNER G.C. , HEATON B., COHEN R.J., DAVIES S.R.
	Mon. Not. R. Astron. Soc., 229, 679-689 (1987)
	Merlin and VLA observations of the star-forming region G 35.2-0.7N.
o	Table 2: <[DLW84] G35.2WN> (No. G35.2N3) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DLZ2016]
[DLZ2016]	(Djupvik+Liimets+Zinnecker+, 2016)
Write:	<<[DLZ2016] MHO NNNN-AN>> <<[DLZ2016] MHO NNNN-AN+N>>
N:	32
Object:	Outflow (SIMBAD class: Outflow)
Stat:	is completely incorporated in Simbad
Note:	NOTCam NIR spectroscopic observations of N=31 H2 emission knots in the field of the Serpens NH3 cloud.
in source:	NAME Serpens NH3
Ref:	=2016A&A...587A..75D
by	DJUPVIK A.A. , LIIMETS T., ZINNECKER H., BARZDIS A., RASTORGUEVA-FOI E.A., PETERSEN L.R.
	Astron. Astrophys., 587A, 75-75 (2016)
	Proper motions of embedded protostellar jets in Serpens.
o	Table 2: <[DLZ2016] MHO NNNN-AN>, <[DLZ2016] MHO NNNN-AN+N> N=32.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DM
DM	(Durchmusterung Nomenclature.)= (RDM)
Write:	<<DM +DD NNNNNA>>
Object:	* (SIMBAD class: Star)
Note:	Durchmusterung Nomenclature, first introduced in the HD catalogue (2nd column): DM eq. BD for stars north of Dec (1875) = -23deg. DM eq. CD for -23deg > Dec(1875) > -52deg. DM eq. CPD (Cape) for stars south of -52deg. See BD, CD or CPD, 900000 stars Catalogues I/83/ and I/84/ are superseded by I/122/
Ref:	=1886BD....C......0S
by	SCHOENFELD E.
	Eds Marcus and Weber's Verlag, Bonn, 0-None (1886)
	Bonner Durchmusterung des sudlichen Himmels.
o	<BD+DD NNNNNA> N=134833.
Ref:	=1903BD....C......0A
by	ARGELANDER F.
	Eds Marcus and Weber's Verlag, Bonn, 0-None (1903)
	Bonner Durchmusterung des nordlichen Himmels.
o	revised by KUSTNER F.
o	<BD+DD NNNNNA>
Ref:	=1892RNAO...16....1T
by	THOME J.M.
	Results of National Argentine Obs., 16, 1-604 (1892)
	Cordoba Durchmusterung declination -22 to -32.
o	<CD +DD NNNNNA> N=179800.
Ref:	=1894RNAO...17....1T
by	THOME J.M.
	Results of National Argentine Obs., 17, 1-538 (1894)
	Cordoba Durchmusterung declination -32 to -42.
o	<CD +DD NNNNNA> N=160415.
Ref:	=1900RNAO...18....1T
by	THOME J.M.
	Results of National Argentine Obs., 18, 1-502 (1900)
	Cordoba Durchmusterung declination -42 to -52.
o	<CD +DD NNNNNA> N=149447.
Ref:	=1914RNAO...21....1T
by	THOME J.M.
	Results of National Argentine Obs., 21, 1-305 (1914)
	Cordoba Durchmusterung declination -52 to -62.
o	<CD +DD NNNNNA> N=about 18000.
Ref:	=1932RNAO...21....1P
by	PERRINE C.D.
	Results of National Argentine Obs., 21, 1-140 (1932)
	Cordoba Durchmusterung declination -62 to -90.
o	<CD +DD NNNNNA> N=about 7800.
Ref:	=1896AnCap...3....1G
by	GILL D. , KAPTEYN J.C.
	Ann. Cape Obs., 3, 1-None (1896)
	Cape photographic Durchmusterung for the equinox 1875 (-18 to -37).
o	<CPD -DD NNNNN>
Ref:	=1897AnCap...4....1G
by	GILL D. , KAPTEYN J.C.
	Ann. Cape Obs., 4, 1-None (1897)
	Cape photographic Durchmusterung for the equinox 1875 (-38 to -52).
o	<CPD -DD NNNNN>
Ref:	=1900AnCap...5....1G
by	GILL D. , KAPTEYN J.C.
	Ann. Cape Obs., 5, 1-None (1900)
	Cape photographic Durchmusterung for the equinox 1875 (-53 to -89).
o	<CPD -DD NNNNN>
Ref:	=1903AnCap...9....1G
by	GILL D.
	Ann. Cape Obs., 9, 1-None (1903)
	Revision of the Cape photographic Durchmusterung for the equinox 1875.
o	<CPD -DD NNNNN>
=E=	Catalogue in electronic form as I/83
=E=	Catalogue in electronic form as I/84
=E=	Catalogue in electronic form as I/119
=E=	Catalogue in electronic form as I/122
=E=	Catalogue in electronic form as I/83
=E=	Catalogue in electronic form as I/84
=E=	Catalogue in electronic form as I/119
=E=	Catalogue in electronic form as I/122
=E=	Catalogue in electronic form as I/114
=E=	Catalogue in electronic form as I/108
Details on Acronym: [DM2015]
[DM2015]	(De Bruyn+MacQuart, 2015) (Not yet in Simbad)
Write:	<<[DM2015] SN>>
N:	6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	WSRT observations of N=6 compact radio sources in the field of QSO J1819+3845.
Ref:	=2015A&A...574A.125D
by	DE BRUYN A.G. , MacQUART J.-P.
	Astron. Astrophys., 574A, 125-125 (2015)
	The intra-hour variable quasar J1819+3845: 13-year evolution, jet polarization structure, and interstellar scattering screen properties.
o	Fig. 12, Table 3: <[DM2015] SN> (Nos S0-S5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DM98]
[DM98]	(Duc+Mirabel, 1998)
Write:	<<[DM98] A>> <<[DM98] Knot a>> <<[DM98] N>>
N:	3+11+2
Object:	G + Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Fig.3a: (Nos A-C), N=3 objects for which spectra was obtained in NGC 5291 region. Fig.3a, Table 3: 'Knot a', N=11 optical knots in NGC 5291 Fig.3a: (Nos 1-2), N=2 background galaxies
in source:	NGC 5291
Ref:	=1998A&A...333..813D
by	DUC P.-A. , MIRABEL I.F.
	Astron. Astrophys., 333, 813-826 (1998)
	Young tidal dwarf galaxies around the gas-rich disturbed lenticular NGC 5291.
o	[DM98] Knot i = CTS K09.09
o	Fig.3a: <[DM98] A> (Nos A-C). Fig.3a, Table 3: <[DM98] Knot a> (Nos a-k). Fig.3a: <[DM98] N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DM99]
[DM99]	(Dolan+Mathieu, 1999)= ([DM99a]) = (lam Ori)
Write:	<<[DM99] NNN>> <<[DM99] JHHMMSS.s+DDMMSS>>
N:	266
Object:	PMS* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	KPNO 0.9m telescope photometry and WIYN spectroscopy of the lam Ori Region.
in source:	NAME lam Ori Region
Ref:	=1999AJ....118.2409D
by	DOLAN C.J. , MATHIEU R.D.
	Astron. J., 118, 2409-2423 (1999)
	A WIYN lithium survey for young stars in the λ Orionis star-forming region.
o	Table 1: <[DM99] NN> (Nos 1-72).
Ref:	=2001AJ....121.2124D
by	DOLAN C.J. , MATHIEU R.D.
	Astron. J., 121, 2124-2147 (2001)
	The spatial distribution of the λ Orionis pre-main-sequence population.
o	Par. 6.2, HD 38361 misprint for 36861 ?
o	Tables 1, 2: <[DM99] NNN> (Nos 73-266) added = <[DM99] JHHMMSS.s+DDMMSS> N=266.
=E=	Catalogue in electronic form as J/AJ/118/2409
=E=	Catalogue in electronic form as J/AJ/121/2124
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DM99a]
[DM99a]	(Dolan+Mathieu, 1999)
*****	Avoid the usage of [DM99a], prefer [DM99]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DM99b]
[DM99b]	(Dos Santos+Mamon, 1999) (Not yet in Simbad)
Write:	<<[DM99b] CN>> <<[DM99b] CNA>>
N:	5+4
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT PSPC observations of HCG 16. N=5 regions of diffuse X-ray emission, (Nos C1-C5). N=4 X-ray sources in C1 region, Nos C1A-C1D).
in source:	HCG 16
Ref:	=1999A&A...352....1D
by	DOS SANTOS S. , MAMON G.A.
	Astron. Astrophys., 352, 1-18 (1999)
	Clumpy diffuse X-ray emission from the spiral-rich compact galaxy group HCG 16.
o	Fig.2: <[DM99b] CN> (Nos C1-C5), <[DM99b] CNA> (Nos C1A-C1D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMA2000]
[DMA2000]	(Del Burgo+Mediavilla+Arribas, 2000) (Not yet in Simbad)
Write:	<<[DMA2000] A>>
N:	8
Object:	Cloud (SIMBAD class: Cloud)
Note:	Map Fig.9 of 8 cloud or regions of ionised gaz in M 31.
in source:	M 31 = NGC 224
Ref:	=2000ApJ...540..741D
by	DEL BURGO C. , MEDIAVILLA E., ARRIBAS S.
	Astrophys. J., 540, 741-754 (2000)
	High-ionization clouds in the circumnuclear region of M31.
o	Table 3: <[DMA2000] A> (Nos a-g).
Details on Acronym: [DMA2007]
[DMA2007]	(Devi+Misra+Agrawal+, 2007)
Write:	<<[DMA2007] JHHMMSS.ss+DDMMSS.ss>>
N:	365
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Point sources in Chandra observations of 30 nearby galaxies.
Ref:	=2007ApJ...664..458D
by	DEVI A.S. , MISRA R., AGRAWAL V.K., SINGH K.Y.
	Astrophys. J., 664, 458-466 (2007)
	The dependence of the estimated luminosities of ultraluminous X-ray sources on spectral models.
o	Table 3: <[DMA2007] JHHMMSS.ss+DDMMSS.ss> N=365.
=E=	Catalogue in electronic form as J/ApJ/664/458
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMA88]
[DMA88]	(Dent+Macdonald+Andersson, 1988)
Write:	<<[DMA88] HII WN>>
N:	5
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
in source:	Onsala 2
Ref:	=1988MNRAS.235.1397D
by	DENT W.R.F. , MacDONALD G.H., ANDERSSON M.
	Mon. Not. R. Astron. Soc., 235, 1397-1410 (1988)
	Observations of the young stellar associations ON2.
o	ON2C=Onsala 2C, ON2S=Onsala 2S.
o	Table II: <[DMA88] HII S>, <[DMA88] HII C>, <[DMA88] HII N>, <[DMA88] HII N1>, <[DMA88] HII N2>, N=5
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMA99]
[DMA99]	(Deutsch+Margon+Anderson+, 1999)
Write:	<<[DMA99] Star A>>
N:	2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	HST NICMOS observations. N=2 stars in the field of GX 17+2. Both are possible optical counterparts of GX 17+2. Map in Fig.2.
Ref:	=1999ApJ...524..406D
by	DEUTSCH E.W. , MARGON B., ANDERSON S.F., WACHTER S., GOSS W.M.
	Astrophys. J., 524, 406-413 (1999)
	Infrared candidates for the intense galactic X-ray source GX 17+2.
o	Table 2: <[DMA99] Star A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMB2006]
[DMB2006]	(Della Valle+Mazzei+Bettoni+, 2003)
Write:	<<[DMB2006] 3-NNA>> <<[DMB2006] 3-NNAN>>
N:	109+13
Object:	G + * (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ISOCAM observations of [ACM2000] sources: N=109 galaxies + 13 stars are identified.
Ref:	=2006A&A...454..453D
by	DELLA VALLE A. , MAZZEI P., BETTONI D., AUSSEL H., DE ZOTTI G.
	Astron. Astrophys., 454, 453-458 (2006)
	A multi-wavelength study of the IRAS Deep Survey galaxy sample. I. Optical observations. The redshift distribution.
o	Table C1: <[DMB2006] 3-NNA>, <[DMB2006] 3-NNAN>, N=109.
=E=	Catalogue in electronic form as J/A+A/454/453
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMB2012]
[DMB2012]	(DE BUIZER+MORRIS+BECKLIN+, 2012)
Write:	<<[DMB2012] SOF1>>
N:	1
Note:	SOFIA FORCAST observations of the field of Orion-BN.
in source:	NAME Orion BN/KL
Ref:	=2012ApJ...749L..23D
by	DE BUIZER J.M. , MORRIS M.R., BECKLIN E.E., ZINNECKER H., HERTER T.L., ADAMS J.D., SHUPING R.Y., VACCA W.D.
	Astrophys. J., 749L, 23 (2012)
	First science observations with SOFIA/FORCAST: 6-37 µm imaging of Orion BN/KL.
o	Table 1: <[DMB2012] SOF1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMB2017]
[DMB2017]	(Dunlop+Mclure+Biggs+, 2017)
Write:	<<[DMB2017] UDFNN>>
N:	16
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ALMA 1.3mm continuum observations of N=16 sources in the Hubble Ultra Deep Field (HUDF).
in source:	NAME Hubble Ultra Deep Field
Ref:	=2017MNRAS.466..861D
by	DUNLOP J.S. , McLURE R.J., BIGGS A.D., GEACH J.E., MICHALOWSKI M.J., IVISON R.J., RUJOPAKARN W., VAN KAMPEN E., KIRKPATRICK A., POPE A., SCOTT D., SWINBANK A.M., TARGETT T.A., ARETXAGA I., AUSTERMANN J.E., BEST P.N., BRUCE V.A., CHAPIN E.L., CHARLOT S., CIRASUOLO M., COPPIN K., ELLIS R.S., FINKELSTEIN S.L., HAYWARD C.C., HUGHES D.H., IBAR E., JAGANNATHAN P., KHOCHFAR S., KOPROWSKI M.P., NARAYANAN D., NYLAND K., PAPOVICH C., PEACOCK J.A., RIEKE G.H., ROBERTSON B., VERNSTROM T., VAN DER WERF P.P., WILSON G.W., YUN M.
	Mon. Not. R. Astron. Soc., 466, 861-883 (2017)
	A deep ALMA image of the Hubble Ultra Deep Field.
o	Tables 2,4: <[DMB2017] UDFNN> (Nos 1-16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DMC
DMC	(Diffuse Molecular Cloud) (Not yet in Simbad)
Write:	<<DMC GLLL.ll+BB.bb>>
N:	100
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	Molecular line data in the Gum nebula region.
Ref:	=2001MNRAS.325.1213W
by	WOERMANN B. , GAYLARD M.J., OTRUPCEK R.
	Mon. Not. R. Astron. Soc., 325, 1213-1227 (2001)
	Kinematics of the Gum nebula region.
o	Table 3: <DMC GLLL.ll+BB.bb> N=100.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DMC2009]
[DMC2009]	(D'Avanzo+Malesani+Covino+, 2009)
Write:	<<[DMC2009] JHHMMSS.ss+DDMMSS.s>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Note:	ESO VLT FORS1/2 and ISAAC observations of the fields of GRB 051227 and GRB 071227.
Ref:	=2009A&A...498..711D
by	D'AVANZO P. , MALESANI D., COVINO S., PIRANOMONTE S., GRAZIAN A., FUGAZZA D., MARGUTTI R., D'ELIA V., ANTONELLI L.A., CAMPANA S., CHINCARINI G., DELLA VALLE M., FIORE F., GOLDONI P., MAO J., PERNA R., SALVATERRA R., STELLA L., STRATTA G., TAGLIAFERRI G.
	Astron. Astrophys., 498, 711-721 (2009)
	The optical afterglows and host galaxies of three short/hard γ-ray bursts.
o	Paragr. 3.1, 5.1: <[DMC2009] JHHMMSS.ss+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMD2004]
[DMD2004]	(De Naray+McGaugh+De Block, 2004) (Not yet in Simbad)
Write:	<<[DMD2004] FNNN-N N>> <<[DMD2004] UGC NNNN N>> <<[DMD2004] UGC 12695 (N)N>>
N:	3+1+5+2+2+7
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	William Herschel Telescope at La Palma spectra of HII regions in Low Brightness Galaxies.
in source:	LSB F563-1
in source:	LSB F571-5
in source:	UGC 1230
in source:	UGC 5005
in source:	UGC 9024
in source:	UGC 12695
Ref:	=2004MNRAS.355..887K
by	KUZIO DE NARAY R. , McGAUGH S.S., DE BLOK W.J.G.
	Mon. Not. R. Astron. Soc., 355, 887-898 (2004)
	Oxygen abundances and chemical evolution in low surface brightness galaxies.
o	Figs 2, Tables 2, 3: <[DMD2004] FNNN-N N> N=3+1, <[DMD2004] UGC NNNN N> N=5+2+2, <[DMD2004] UGC 12695 (N)N> N=3+4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMD2005]
[DMD2005]	(De Rijcke+Michielsen+Dejonghe+, 2005)
Write:	<<[DMD2005] NGC 5898 DWN>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 imaging spectrograph observations of dwarf elliptical galaxies. N=2 new objects are found.
Ref:	=2005A&A...438..491D
by	DE RIJCKE S. , MICHIELSEN D., DEJONGHE H., ZEILINGER W.W., HAU G.K.T.
	Astron. Astrophys., 438, 491-505 (2005)
	Formation and evolution of dwarf elliptical galaxies. I. Structural and kinematical properties.
o	Table 1: <[DMD2005] NGC 5898 DWN> (Nos DW1-DW2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMD2008]
[DMD2008]	(Drake Mahabal Djorgovski+, 2008)
Write:	<<[DMD2008] JHHMMSS.ss+DDMMSS.s>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Catalina Schmidt Telescope observations. Host galaxies of SN 2008dc, SN 2008de, SN 2008dg.
Ref:	=2008CBET.1409....1D
by	DRAKE A.J. , MAHABAL A., DJORGOVSKI S.G., GRAHAM M.J., WILLIAMS R., BESHORE E.C., LARSON S.M., CHRISTENSEN E.
	CBET, 1409, 1 (2008)
	Supernovae 2008dc, 2008dd, 2008de, 2008df, 2008dg, 2008dh, 2008di.
o	<[DMD2008] JHHMMSS.ss+DDMMSS.s> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMD2011]
[DMD2011]	(Dawson+McClure-Griffiths+Dickey+, 2011)
Write:	<<[DMD2011] A>>
N:	3
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	Mopra 12CO(1-0) and 13CO(1-0) observations of walls of Galactic supershells.
Ref:	=2011ApJ...741...85D
by	DAWSON J.R. , McCLURE-GRIFFITHS N.M., DICKEY J.M., FUKUI Y.
	Astrophys. J., 741, 85 (2011)
	Molecular clouds in supershells: a case study of three objects in the walls of GSH 287+04-17 and GSH 277+00+36.
o	Figs 1-3, Table 1: <[DMD2011] A> (Nos A-C).
o	Region D is not in SIMBAD.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMD2023]
[DMD2023]	(Donnan+McLeod+Dunlop+, 2023)
Write:	<<[DMD2023] COSMOS-NNNNNN>> <<[DMD2023] SMACS-NNNNN>> <<[DMD2023] CEERS-NNNNNN>> <<[DMD2023] CEERS-NNNNN-N>> <<[DMD2023] GLASS-NNNNN>>
N:	16+23+9+10+3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=16 galaxies in the COSMOS field and N=45 galaxies in three JWST fields. Use of UltraVISTA DR5 in the COSMOS field and JWST archival data from ERO and ERS programs (SMACS J0723 cluster, CEERS and GLASS).
Ref:	=2023MNRAS.518.6011D
by	DONNAN C.T. , McLEOD D.J., DUNLOP J.S., McLURE R.J., CARNALL A.C., BEGLEY R., CULLEN F., HAMADOUCHE M.L., BOWLER R.A.A., MAGEE D., McCRACKEN H.J., MILVANG-JENSEN B., MONETI A., TARGETT T.
	Mon. Not. R. Astron. Soc., 518, 6011-6040 (2023)
	The evolution of the galaxy UV luminosity function at redshifts z ≃ 8 - 15 from deep JWST* and ground-based near-infrared imaging.*
o	Tables 3+B1: <[DMD2023] COSMOS-NNNNNN> N=16 among (Nos 306122-978389). Tables 5+B2: <[DMD2023] SMACS-NNNNN> N=23 among (Nos 1566-44711), <[DMD2023] CEERS-NNNNNN> N=9 among (Nos 1698-127682), <[DMD2023] CEERS-NNNNN-N> N=10 among (Nos 622-4 to 33593-2), <[DMD2023] GLASS-NNNNN> (Nos 1698, 6415, 17487).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [DME94]
[DME94]	(Davis+Mundt+Eisloffel, 1994)
Write:	<<[DME94] HH 110 IRS N>> <<[DME94] HH 111 IRS>> <<[DME94] HH 111 CJN>>
N:	2+1+3
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	(IR) in HH 110 and HH 111. 3 new knots are added in the HH 111 CounterJet (Nos CJ1-CJ3)
in source:	HH 110
in source:	HH 111
Ref:	=1994ApJ...437L..55D
by	DAVIS C.J. , MUNDT R., EISLOEFFEL J.
	Astrophys. J., 437, 55-58 (1994)
	Near-infrared imaging of the jets and flows associated with Herbig-Haro objects HH 91, HH 110 and HH 111.
o	Plates: stars 'NN' are '[RO91] NN'
o	Fig.3: <[DME94] HH 110 IRS N> (Nos 1-2). Fig.5: <[DME94] HH 111 IRS>N=1. Fig.5: <[DME94] HH 111 CJN> (Nos CJ1 to CJ3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DME98]
[DME98]	(Davis+Moriarty-Schieven+Eisloffel+, 1998)
Write:	<<[DME98] AFGL 490 IRS>> <<[DME98] AFGL 490 Knot A>> <<[DME98] S140N ZN>> <<[DME98] AFGL 5180 Centre A>> <<[DME98] AFGL 5180 Centre WN>> <<[DME98] AFGL 5180 East A>>
N:	2+2+14
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Note:	Table 1, Fig.1: N=1 IRS in AFGL 490, and N=1 Knot 'A'. Fig.5: N=2 counterflows Z1 and Z2 in Sh 2-140N. Fig.9: N=4 Knots (Nos A-D) in the Centre of AFGL 5180, N=3 features 'N', S1, and 'S2' Fig.10: N=7 Knots (Nos A-G) in the eastern jet of AFGL 5180.
in source:	RAFGL 490
in source:	SH 2-140 N
in source:	RAFGL 5180
Ref:	=1998AJ....115.1118D
by	DAVIS C.J. , MORIARTY-SCHIEVEN G., EISLOEFFEL J., HOARE M.G., RAY T.P.
	Astron. J., 115, 1118-1134 (1998)
	Observations of shocked H_2 and entrained CO in outflows from luminous young stars.
o	<HH NNN> (Nos 251-254). Table 1, Fig.1: <[DME98] AFGL 490 IRS> N=1, < [DME98] AFGL 490 Knot A> N=1. Fig.5: <[DME98] S140N ZN> (Nos Z1-Z2). Fig.9: <[DME98] AFGL 5180 Centre A> (Nos A-D), <[DME98] AFGL 5180 Centre WN> (Nos N, S1, S2). Fig.10: <[DME98] AFGL 5180 East A> (Nos A-G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMG2002]
[DMG2002]	(Dieball+Muller+Grebel+, 2002)
Write:	<<[DMG2002] NNN>>
N:	473
Object:	Group of stellar clusters (SIMBAD class: Cluster* = Cluster of Stars)
Note:	N=473 binaries and multiple stellar clusters in the LMC, from the BSDL catalogue.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2002A&A...391..547D
by	DIEBALL A. , MUELLER H., GREBEL E.K.
	Astron. Astrophys., 391, 547-564 (2002)
	A statistical study of binary and multiple clusters in the LMC.
o	Multiple clusters have not been integrated into Simbad. The clusters Rob1 and U1 have not been found.
o	Table 6: <[DMG2002] NNN> (Nos 1-473).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMG2011]
[DMG2011]	(Da Rocha+Mieske+Georgiev+, 2011)
Write:	<<[DMG2011] HCGNN UCDNN>> <<[DMG2011] HCGNN_UCDNNN>> (not recognised by Simbad, but found in literature)
N:	16+5
Object:	Compact Stellar System (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 observations of N=16+5 compact stellar systems in HCG 22 and HCG 90, respectively. Use of archival HST ACS imaging.
Ref:	=2011A&A...525A..86D
by	DA ROCHA C. , MIESKE S., GEORGIEV I.Y., HILKER M., ZIEGLER B.L., MENDES DE OLIVEIRA C.
	Astron. Astrophys., 525A, 86-86 (2011)
	Two formation channels of ultra-compact dwarf galaxies in Hickson compact groups.
o	Tables 1, 3: <[DMG2011] HCG22 UCDNN> (Nos 1-16). Tables 2, 4: <[DMG2011] HCG90 UCDN> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMH2015]
[DMH2015]	(Dekany+Minniti+Hajdu+, 2015)
Write:	<<[DMH2015] CN>>
N:	2
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Stat:	is completely incorporated in Simbad
Note:	NIR photometry of N=2 classical Cepheid stars located in the Galactic plane behind the bulge. Use of data from the ESO Public Survey "VISTA Variables in the Via Lactea" (VVV).
Ref:	=2015ApJ...799L..11D
by	DEKANY I. , MINNITI D., HAJDU G., ALONSO-GARCIA J., HEMPEL M., PALMA T., CATELAN M., GIEREN W., MAJAESS D.
	Astrophys. J., 799L, 11 (2015)
	Discovery of a pair of classical cepheids in an invisible cluster beyond the galactic bulge.
o	Table 1:<[DMH2015] CN> (Nos C1-C2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMH96]
[DMH96]	(Dring+Murthy+Henry+, 1996)
Write:	<<[DMH96] NNN>>
N:	194
Object:	Dust Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	A early work in 1992ApJ...401..574M, containing N=123 clouds, is superseded by 1996ApJ...457..764D. N=194 clouds around 138 stars.
Ref:	=1996ApJ...457..764D
by	DRING A.R. , MURTHY J., HENRY R.C., WALKER H.J.
	Astrophys. J., 457, 764-772 (1996)
	The distribution of dust clouds in the interstellar medium.
o	An early work in 1992ApJ...401..574M, containing N=123 clouds, is now superseded by this work.
o	Table 1, col(1): <[DMH96] NNN> (Nos 1-194)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMJ2015]
[DMJ2015]	(Dutta+Mondal+Jose+, 2015)
Write:	<<[DMJ2015] NNNN>>
N:	5601
Object:	* (SIMBAD class: Star)
Note:	2m Himalayan Chandra telescope and 1.04m Sampurnanand telescope spectrophotometric observations of N=5601 stars in the field of the young cluster NGC 2282. Use of archival IPHAS, 2MASS, UKIDSS and Spitzer IRAC data.
in source:	NGC 2282
Ref:	=2015MNRAS.454.3597D
by	DUTTA S. , MONDAL S., JOSE J., DAS R.K., SAMAL M.R., GHOSH S.
	Mon. Not. R. Astron. Soc., 454, 3597-3612 (2015)
	The young cluster NGC 2282: a multiwavelength perspective.
o	Table 2: <[DMJ2015] NNNN> (Nos 1-5601).
=E=	Catalogue in electronic form as J/MNRAS/454/3597
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMJ2019]
[DMJ2019]	(Dutta+Mondal+Joshi+, 2019)
Write:	<<[DMJ2019] NNNN>>
N:	31
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	ARIES 1.3m Devasthal Fast Optical Telescope (DFOT) and ARIES 1.04m Sampurnanand telescope (both in Nainital, India), and Himalayan Chandra 2m telescope (HCT, India) HFOSC observations of N=31 variable stars towards the star-forming region Cygnus OB7. Use of UKIDSS and WISE data.
in source:	Ass Cyg OB 7
Ref:	=2019MNRAS.487.1765D
by	DUTTA S. , MONDAL S., JOSHI S., DAS R.
	Mon. Not. R. Astron. Soc., 487, 1765-1776 (2019)
	Optical photometric variable stars towards Cygnus OB7.
o	Tables 2-3: <[DMJ2019] NNNN> N=31 among (Nos 8-6927).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMJ2020]
[DMJ2020]	(Dempsey+McClure-Griffiths+Jameson+, 2020) (Not yet in Simbad)
Write:	<<[DMJ2020] SUMSS J012734-713639A>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ATCA observations of N=2 components of SUMSS J012734-713639.
Ref:	=2020MNRAS.496..913D
by	DEMPSEY J. , McCLURE-GRIFFITHS N.M., JAMESON K., BUCKLAND-WILLIS F.
	Mon. Not. R. Astron. Soc., 496, 913-920 (2020)
	Cold H I ejected into the Magellanic Stream.
o	Fig. 5, Table 1: <[DMJ2020] SUMSS J012734-713639A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMJ93]
[DMJ93]	(DeGioia-Eastwood+Meyers+Jones, 1993)
Write:	<<[DMJ93] LH 13 NNN>>
N:	154
Object:	* (SIMBAD class: Star)
Note:	Table 3: * in LH 13, format 'LH 13 NNN', N=154.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1993AJ....106.1005D
by	DEGIOIA-EASTWOOD K. , MEYERS R.P., JONES D.P.
	Astron. J., 106, 1005-1023 (1993)
	Luminosity functions and color-magnitude diagrams for three OB associations in the Large Magellanic Cloud.
o	Table 3: <[DMJ93] LH 13 NNN> N=154, Table 4: <[DMJ93] LH 76 NNN> N=222 ,Table 5: <[DMJ93] LH 105 N NNN> N=123, Table 6: <[DMJ93] LH 105 S NNN> N=101
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMJ93]
[DMJ93]	(DeGioia-Eastwood+Meyers+Jones, 1993)
Write:	<<[DMJ93] LH 76 NNN>> <<[DMJ93] LH 105 W NNN>>
N:	222+224
Object:	* (SIMBAD class: Star)
Note:	Table 4: * in LH 76, format 'LH 76 NNN', N=222. Table 4: * in LH 105 North, format 'LH 105 W NNN', with 'W' = N for North, N=123. Table 5: * in LH 105 South, format 'LH 105 W NNN', with 'W' = S for South, N=101.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1993AJ....106.1005D
by	DEGIOIA-EASTWOOD K. , MEYERS R.P., JONES D.P.
	Astron. J., 106, 1005-1023 (1993)
	Luminosity functions and color-magnitude diagrams for three OB associations in the Large Magellanic Cloud.
o	Table 3: <[DMJ93] LH 13 NNN> N=154, Table 4: <[DMJ93] LH 76 NNN> N=222 ,Table 5: <[DMJ93] LH 105 N NNN> N=123, Table 6: <[DMJ93] LH 105 S NNN> N=101
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMK92]
[DMK92]	(Djorgovski+Meylan+Klemola+, 1992)
Write:	<<[DMK92] AA>>
N:	23+6
Object:	* + (Rad) + Opt. Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 1: field stars, N=23 among (Nos A-Z). Table 2: Radio and optical candidates, N=6.
Ref:	=1992MNRAS.257..240D
by	DJORGOVSKI S. , MEYLAN G., KLEMOLA A., THOMPSON D.J., WEIR W.N., SWARUP G., RAO A.P., SUBRAHMANYAN R., SMETTE A.
	Mon. Not. R. Astron. Soc., 257, 240-244 (1992)
	A search for the optical/IR counterpart of the probable Einstein ring source 1830-211.
o	Table 1: <[DMK92] A> N=23, Table 2: <[DMK92] AA> N=6
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMK97]
[DMK97]	(Djorgovski+Metzger+Kukarni+, 1997)
Write:	<<[DMK97] gN>> <<[DMK97] Star A>>
N:	1+2
Object:	G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Finding chart of the field of GRB 970508: N=1 galaxie, 'g1' = [NBS97] G1 = [PFB98] G1. N=2 stars 'A' and 'N'. See also [NBS97], [PFB98], and [ZSB98]
Ref:	=1997Natur.387..876D
by	DJORGOVSKI S.G. , METZGER M.R., KULKARNI S.R., ODEWAHN S.C., GAL R.R., PAHRE M., FRAIL D.A., FEROCI M., COSTA E., PALAZZI E.
	Nature, 387, 876-878 (1997)
	The optical counterpart to the γ-ray burst GRB 970508.
o	OT = [NBS97] OT
o	<[DMK97] g1> N=1, <[DMK97] Star A> (Nos A, N).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DML2018]
[DML2018]	(Di Teodoro+McClure-Griffiths+Lockman+, 2018)
Write:	<<[DML2018] GLLL.l+BB.b+VVV>>
N:	106
Object:	HI (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	GBT HI observations of N=106 compact clouds above and below the Galactic Center (up to Galactic latitude \|b\|<10°). See also [MGH2013], [LDM2020].
Ref:	=2018ApJ...855...33D
by	DI TEODORO E.M. , McCLURE-GRIFFITHS N.M., LOCKMAN F.J., DENBO S.R., ENDSLEY R., FORD H.A., HARRINGTON K.
	Astrophys. J., 855, 33-33 (2018)
	Blowing in the Milky Way wind: neutral hydrogen clouds tracing the Galactic nuclear outflow.
o	Tables 1-2: <[DML2018] GLLL.l+BB.b+VVV> N=106.
=E=	Catalogue in electronic form as <J/ApJ/855/33/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DML2020]
[DML2020]	(Di Teodoro+McClure-Griffiths+Lockman+, 2020)
Write:	<<[DML2020] MW-CN>>
N:	2
Object:	Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	APEX 12CO(2-1) observations of N=2 clouds near the Galactic center.
Ref:	=2020Natur.584..364D
by	DI TEODORO E.M. , McCLURE-GRIFFITHS N.M., LOCKMAN F.J., ARMILLOTTA L.
	Natur, 584, 364-367 (2020)
	Cold gas in the Milky Way's nuclear wind.
o	Table 1: <[DML2020] MW-CN> (Nos MW-C1, MW-C2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DML87]
[DML87]	(De Grijp+Miley+Lub, 1987)
Write:	<<[DML87] NNN>>
N:	749
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Ref:	=1987A&AS...70...95D
by	DE GRIJP M.H.K. , MILEY G.K., LUB J.
	Astron. Astrophys., Suppl. Ser., 70, 95-114 (1987)
	Warm IRAS sources. I. A catalogue of AGN candidates from the point source catalog.
o	Tables I to III: <[DML87] NNN> (Nos 1-563, 564-740, 741-749).
=E=	Catalogue in electronic form as J/A+AS/70/95
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMM2003]
[DMM2003]	(Davis+Miller+Mushotzky, 2003)
Write:	<<[DMM2003] N>>
N:	8
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of 8 galaxies in ACO 2255, associated with point-like X-ray emission.
in source:	ACO 2255
Ref:	=2003ApJ...597..202D
by	DAVIS D.S. , MILLER N.A., MUSHOTZKY R.F.
	Astrophys. J., 597, 202-209 (2003)
	Chandra observations of point sources in A2255.
o	Table 1: <[DMM2003] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMM2008]
[DMM2008]	(Desert+Macias-Perz+Mayet+, 2007)= ([DMM2008a])
Write:	<<[DMM2008] NNN>>
N:	302
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	Archeops balloon-borne experiment by-product: smm catalog of bright smm point sources. See Arch.
Ref:	=2008A&A...481..411D
by	DESERT F.-X. , MACIAS-PEREZ J.F., MAYET F., GIARDINO G., RENAULT C., AUMONT J., BENOIT A., BERNARD J.-P., PONTHIEU N., TRISTRAM M.
	Astron. Astrophys., 481, 411-421 (2008)
	Submillimetre point sources from the Archeops experiment: very cold clumps in the Galactic plane.
o	Table 3, col(1): <[DMM2008] NNN> (Nos 1-302) = Table 3, col(2): <Arch GLLL.ll+BB.bb> N=302.
=E=	Catalogue in electronic form as J/A+A/481/411
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMM2008a]
[DMM2008a]	(Desert+Macias-Perz+Mayet+, 2007)
*****	Avoid the usage of [DMM2008a], prefer [DMM2008]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMM2008b]
[DMM2008b]	(Diaz-Gimenez+Muriel+Mendez De Oliveira, 2008)
Write:	<<[DMM2008b] R>>
N:	6
Object:	Fossil Group (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=6 candidate fossil groups in the SDSS DR6.
Ref:	=2008A&A...490..965D
by	DIAZ-GIMENEZ E. , MURIEL H., MENDES DE OLIVEIRA C.
	Astron. Astrophys., 490, 965-973 (2008)
	Fossil groups in the Millennium Simulation. Evolution of the brightest galaxies.
o	Table 5 : <[DMM2008b] R> (Nos I-VI).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMM2009]
[DMM2009]	(Drout+Massey+Meynet+, 2009)
Write:	<<[DMM2009] JHHMMSS.ss+DDMMSS.s>>
N:	2629
Object:	Star (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	MMT Hectospec observations of M31 yellow supergiants.
Ref:	=2009ApJ...703..441D
by	DROUT M.R. , MASSEY P., MEYNET G., TOKARZ S., CALDWELL N.
	Astrophys. J., 703, 441-460 (2009)
	Yellow supergiants in the Andromeda galaxy (M31).
o	Tables 3-5: <[DMM2009] JHHMMSS.ss+DDMMSS.s> N=2629.
=E=	Catalogue in electronic form as <J/ApJ/703/441/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMM2015]
[DMM2015]	(Dekany+Minniti+Majaess+, 2015)
Write:	<<[DMM2015] NN>>
N:	35
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Stat:	is completely incorporated in Simbad
Note:	NIR photometry of N=35 classical Cepheid stars in the central region of the Galaxy. Use of data from the ESO Public Survey "VISTA Variables in the Via Lactea" (VVV).
Ref:	=2015ApJ...812L..29D
by	DEKANY I. , MINNITI D., MAJAESS D., ZOCCALI M., HAJDU G., ALONSO-GARCIA J., CATELAN M., GIEREN W., BORISSOVA J.
	Astrophys. J., 812L, 29 (2015)
	The VVV survey reveals classical cepheids tracing a young and thin stellar disk across the galaxy's bulge.
o	Table 1: <[DMM2015] NN> (Nos 1-35).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMM94]
[DMM94]	(Dickey+Melbold+Marx+, 1994)
Write:	<<[DMM94] JHHMM+DDda>>
N:	30
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Paper I 1991A&A...251L...1M: 5 PKS sources.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1994A&A...289..357D
by	DICKEY J.M. , MEBOLD U., MARX M., AMY S., HAYNES R.F., WILSON W.
	Astron. Astrophys., 289, 357-380 (1994)
	The Australia Telescope Survey of 21-cm absorption in the Magellanic System II. The cool atomic gas in the LMC.
o	Table 1: <[DMM94] JHHMM-DDdA> N=30.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMN2000]
[DMN2000]	(De Vicente+Martin-Pintado+Neri+, 2000)
Write:	<<[DMN2000] Sgr B2 AN>>
N:	2+4
Object:	Hot Core (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=2 hot cores in NAME Sgr B2 (N) region, (Nos N1-N2). N=4 hot cores in the ridge connecting NAME Sgr B2 (M) and (N), (Nos R1-R4).
in source:	NAME Sgr B2
Ref:	=2000A&A...361.1058D
by	DE VICENTE P. , MARTIN-PINTADO J., NERI R., COLOM P.
	Astron. Astrophys., 361, 1058-1072 (2000)
	A ridge of recent massive star formation between Sgr B2M and Sgr B2N.
o	Table 8: <[DMN2000] Sgr B2 AN> (Nos N1-N2, R1-R4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMN2002]
[DMN2002]	(De Vicente+Martin-Pintado+Neri, 2002) (Not yet in Simbad)
Write:	<<[DMN2002] AAN>>
N:	2
Object:	Hot Core (SIMBAD class: PartofCloud = Part of Cloud)
Note:	N=2 peaks in Orion KL Hot Core.
in source:	NAME Orion KL
Ref:	=2002ApJ...574L.163D
by	DE VICENTE P. , MARTIN-PINTADO J., NERI R., RODRIGUEZ-FRANCO A.
	Astrophys. J., 574, 163-166 (2002)
	On the heating source of the Orion KL hot core.
o	Source I = GMR I, source IRc2 = [RLK73] IRc 2.
o	<[DMN2002] HCN> (Nos HC1, HC2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMO2000]
[DMO2000]	(Dohm-Palmer+Mateo+Olszewski+, 2000)
Write:	<<[DMO2000] LLL.ll+BB.bb>>
N:	32655
Object:	* (SIMBAD class: Star)
Note:	Astrometric and photometric catalogue.
Ref:	=2000AJ....120.2496D
by	DOHM-PALMER R.C. , MATEO M., OLSZEWSKI E., MORRISON H., HARDING P., FREEMAN K.C., NORRIS J.
	Astron. J., 120, 2496-2512 (2000)
	Mapping the galactic halo. II. Photometric survey.
o	Table 4: <[DMO2000] LLL.ll+BB.bb> N=32655.
=E=	Catalogue in electronic form as J/AJ/120/2496
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DMOC
DMOC	(Delingha Molecular Otuflow Candidate)
Write:	<<DMOC -NNNN>>
N:	130
Object:	Poss. Outflow (SIMBAD class: Outflow_Candidate = Outflow Candidate)
Note:	Purple Moutain Observatory Delingha 13.7m telescope observations of N=130 outflow candidates across the dark cloud complex in the Cygnus region, as part of the Milky Way Imaging Scroll Painting (MWISP) survey.
in source:	Name Cygnus Region
Ref:	=2020ApJS..248...15Z
by	ZHANG S. , YANG J., XU Y., CHEN X., SU Y., SUN Y., ZHOU X., LI Y., LU D.
	Astrophys. J., Suppl. Ser., 248, 15-15 (2020)
	Searching for molecular outflows with support vector machines: the dark cloud complex in Cygnus.
o	Tables 1-2: <DMOC-NNNN> (Nos 0001-0130).
o	Pelican's Hat, Head and Neck are not in SIMBAD.
=E=	Catalogue in electronic form as <J/ApJS/248/15/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DMP2012]
[DMP2012]	(Diaz-Gimenez+Mamon+Pacheco+, 2012)
Write:	<<[DMP2012] NN>>
N:	85
Object:	Compact Group (SIMBAD class: Compact_Gr_G = Compact Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Photometric catalogue of N=85 compact groups of galaxies (p2MCGs) automatically extracted from the 2MASX source catalogue.
Ref:	=2012MNRAS.426..296D
by	DIAZ-GIMENEZ E. , MAMON G.A., PACHECO M., MENDES DE OLIVEIRA C., ALONSO M.V.
	Mon. Not. R. Astron. Soc., 426, 296-316 (2012)
	Compact groups of galaxies selected by stellar mass: the 2MASS compact group catalogue.
o	Table C1: <[DMP2012] NN> (Nos 1-85).
o	2MASX J11561032+6031211 and 2MASX J14080314-3318542 do not exist in the 2MASX catalog, and are not in Simbad.
=E=	Catalogue in electronic form as J/MNRAS/426/296
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMP2019]
[DMP2019]	(Doroshenko+Malyshev+Puhlhofer+, 2019)
Write:	<<[DMP2019] nN>>
N:	6
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	N=6 sources in the field of SNR G094.0+01.0 (3C 434.1), that are not in the 8yr Fermi LAT catalog (FL8Y).
Ref:	=2019A&A...631A.179D
by	DOROSHENKO V. , MALYSHEV D., PUHLHOFER G., DINCEL B., SASAKI M., SANTANGELO A.
	Astron. Astrophys., 631A, 179-179 (2019)
	XMM-Newton and Fermi/LAT view on the supernova remnant 3C434.1.
o	Fig. 3, Table 2: <[DMP2019] nN> (Nos n1-n6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DMPP
DMPP	(Dispersed Matter Planet Project) (Not yet in Simbad)
Write:	<<DMPP -NAa>> <<DMPP -NA a>> (not recognised by Simbad, but found in literature)
Object:	* + Planet (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Host stars and low-mass planets detected by the Dispersed Matter Planet Project (DMPP).
Ref:	=2020NatAs...4..399S
by	STAAB D. , HASWELL C.A., BARNES J.R., ANGLADA-ESCUDE G., FOSSATI L., DOHERTY J.P.J., COOPER J., JENKINS J.S., DIAZ M.R., SOTO M.G.
	NatAs, 4, 399-407 (2020)
	A compact multi-planet system around a bright nearby star from the Dispersed Matter Planet Project.
o	<DMPP-Na> (Nos 1, 1b-1e).
Ref:	=2020NatAs...4..408H
by	HASWELL C.A. , STAAB D., BARNES J.R., ANGLADA-ESCUDE G., FOSSATI L., JENKINS J.S., NORTON A.J., DOHERTY J.P.J., COOPER J.
	NatAs, 4, 408-418 (2020)
	Dispersed Matter Planet Project discoveries of ablating planets orbiting nearby bright stars.
o	<DMPP-Na> (Nos 2, 2b).
Ref:	=2020NatAs...4..419B
by	BARNES J.R. , HASWELL C.A., STAAB D., ANGLADA-ESCUDE G., FOSSATI L., DOHERTY J.P.J., COOPER J., JENKINS J.S., DIAZ M.R., SOTO M.G., PENA ROJAS P.A.
	NatAs, 4, 419-426 (2020)
	An ablating 2.6 M⊕ planet in an eccentric binary from the Dispersed Matter Planet Project.
o	<DMPP-NAa> (Nos 3, 3A-3B, 3Ab).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DMR2002]
[DMR2002]	(De Vries+Morganti+Rottgering+, 2002)
Write:	<<[DMR2002] JHHMMSS+DDMMSS>>
N:	3172
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	WSRT observations of the Bootes Deep Field.
in source:	NAME Bootes Field
Ref:	=2002AJ....123.1784D
by	DE VRIES W.H. , MORGANTI R., ROETTGERING H.J.A., VERMEULEN R., VAN BREUGEL W., RENGELINK R., JARVIS M.J.
	Astron. J., 123, 1784-1800 (2002)
	Deep Westerbork 1.4 GHz imaging of the Bootes field.
o	Table 2: <[DMR2002] JHHMMSS+DDMMSS> N=3172.
=E=	Catalogue in electronic form as J/AJ/123/1784
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMR99]
[DMR99]	(Davis+Matthews+Ray+, 1999)
Write:	<<[DMR99] Knot a>> <<[DMR99] Extension N>> <<[DMR99] Lobe WWbN>> <<[DMR99] Lobe WWrN>>
N:	3+2+11
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Note:	Table 2, Fig.1: N=3 'Knots' or 'Sub-clumps' (Nos a-c) in the SMM '[CED93] 9'. Fig.1: N=2 'Extensions (Nos 1-2) in the SMM '[CED93] 1'. Fig.4: N=11 'Lobes' or high-velocity CO features in the SMM 1 and 4 ([CED93] 1 amd [CED93] 4) region. in the format 'WWAn', 'WW' stands for directions (including 'C' for 'Center'), the letter 'r' stands red-shifted feature or 'b': blue-shifted feature.
in source:	NAME Serpens Cloud
Ref:	=1999MNRAS.309..141D
by	DAVIS C.J. , MATTHEWS H.E., RAY T.P., DENT W.R.F., RICHER J.S.
	Mon. Not. R. Astron. Soc., 309, 141-152 (1999)
	A burst of outflows from the Serpens cloud core: wide-field submillimetre continuum, CO j = 2-1 and optical observations.
o	SMM NN objects are [CED93] NN in SIMBAD.
o	Table 1: <HH NNN> (Nos 456-457). Table 2, Fig.1: <[DMR99] Knot a> (Nos a-c). Fig.1: <[DMR99] Extension N> (Nos 1-2). Fig.4: <[DMR99] Lobe WWaN> N=11. Table 2: <[CED93] NN> (Nos 10-11) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DMS
DMS	(Drissen+Moffat+Shara)= (WR)
Write:	<<DMS NGC 604 NNa>> <<DMS NGC 604 VN>> <<DMS NGC 595 NNa>> <<DMS NGC 592 N>>
N:	17+1+13+2
Object:	WR (SIMBAD class: WolfRayet* = Wolf-Rayet)
Stat:	is completely incorporated in Simbad
Note:	format 'NGC 604 NNa', (Nos 1-13): the second ref. introduces the format 'NNa' (Nos 2a, 2b, 4a, 4b) and objects Nos 11, 12 are added (table 2, col. WR?) format 'NGC 604 V1': N=1, in 1st ref. Fig 1b, in 2nd ref. table 2, col. WR?. format 'NGC 595 NNa', (Nos 1-11): the second ref. introduces the format 'NNa' (Nos 2a, 2b) format 'NGC 592 N' (Nos 1-2): N=2, 1st ref., Table 6
in source:	M 33:NGC 604 = NGC 604
in source:	M 33:NGC 595 = NGC 595
in source:	M 33:NGC 592 = NGC 592
Ref:	=1990ApJ...364..496D
by	DRISSEN L. , MOFFAT A.F.J., SHARA M.M.
	Astrophys. J., 364, 496-512 (1990)
	The Wolf-Rayet star population in the most massive giant HII regions of M 33.
o	Fig.1: <DMS NGC 604 V1>, Table 4: <DMS NGC 604 NN> N=10, Table 5: <DMS NGC 595 NN> N=11, Table 6: <DMS NGC 592 N> N=2
Ref:	=1993AJ....105.1400D
by	DRISSEN L. , MOFFAT A.F.J., SHARA M.M.
	Astron. J., 105, 1400-1410 (1993)
	A Hubble Space Telescope planetary camera view of giant HII regions: the Wolf-Rayet content of NGC 595 and NGC 604 in M 33.
o	Table 1, col. (1): <[DMS93] NGC 595 NNN> N=113 among 121. Table 1, col. (WR?): <DMS NGC 595 NNa> (Nos 2a, 2b) added. Table 2, col (1): <[DMS93] NGC 604 NNN> N=207 among 254. Table 2, col. (WR?): <DMS NGC 604 NNa> (Nos 2a, 2b, 4a, 4b) added.
Ref:	=2008MNRAS.389.1033D
by	DRISSEN L. , CROWTHER P.A., UBEDA L., MARTIN P.
	Mon. Not. R. Astron. Soc., 389, 1033-1040 (2008)
	Wolf-Rayet stars in M33 - II. Optical spectroscopy of emission-line stars in giant HII regions.
o	Table 2: <DMS NGC 604 NN> (No. 13) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DMS
DMS	(Deep Multicolor Survey)
*****	Avoid the usage of DMS, prefer [HOG96]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DMS2000]
[DMS2000]	(Drake+Merrifield+Sakelliou+, 2000)= ([DMS2000a])
Write:	<<[DMS2000] JHHMMSS+DDMMSS>>
N:	1
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	N=1 example of galaxy member of ACO 160 and associated with an X-ray wake.
in source:	ACO 160
Ref:	=2000MNRAS.314..768D
by	DRAKE N. , MERRIFIELD M.R., SAKELLIOU I., PINKNEY J.C.
	Mon. Not. R. Astron. Soc., 314, 768-774 (2000)
	X-ray wakes in Abell 160.
o	p.769: <[DMS2000] JHHMMSS+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMS2000a]
[DMS2000a]	(Drake+Merrifield+Sakelliou+, 2000)
*****	Avoid the usage of [DMS2000a], prefer [DMS2000]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMS2000b]
[DMS2000b]	(Dickey+Mebold+Stanimirovic+, 2000)
Write:	<<[DMS2000b] JHHMMSS+DDMMSS>>
N:	28
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=13 sources with detected absorption. Table 2: N=15 sources with no absorption detected.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2000ApJ...536..756D
by	DICKEY J.M. , MEBOLD U., STANIMIROVIC S., STAVELEY-SMITH L.
	Astrophys. J., 536, 756-772 (2000)
	Cold atomic gas in the Small Magellanic Cloud.
o	Tables 1, 2: <[DMS2000b] JHHMMSS+DDMMSS> N=13+15.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMS2006]
[DMS2006]	(Damiani+Micela+Sciortino, 2006)= ([DMS2006a])
Write:	<<[DMS2006] NN>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-I observations of the region around the star MWC 297.
Ref:	=2006A&A...447.1041D
by	DAMIANI F. , MICELA G., SCIORTINO S.
	Astron. Astrophys., 447, 1041-1048 (2006)
	Chandra X-ray observations of the stellar group near the Herbig Be star MWC 297. A revision of the X-ray properties of MWC 297.
o	Table 1: <[DMS2006] NN> (Nos 1-27).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMS2006a]
[DMS2006a]	(Damiani+Micela+Sciortino, 2006)
*****	Avoid the usage of [DMS2006a], prefer [DMS2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMS2006b]
[DMS2006b]	(Damiani+Micela+Sciortino+, 2006)
Write:	<<[DMS2006b] NNN>>
N:	387
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS X-ray observations of NGC 2362.
in source:	NGC 2362
Ref:	=2006A&A...460..133D
by	DAMIANI F. , MICELA G., SCIORTINO S., HUELAMO N., MOITINHO A., HARNDEN F.R.Jr, MURRAY S.S.
	Astron. Astrophys., 460, 133-144 (2006)
	The young star cluster NGC 2362: low-mass population and initial mass function from a Chandra X-ray observation.
o	Table 2: <[DMS2006b] NNN> (Nos 1-387).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMS2018]
[DMS2018]	(Dutta+Mondal+Samal+, 2018)
Write:	<<[DMS2018] SNN>> <<[DMS2018] JDDD.ddddd+DD.ddddd>>
N:	5+111
Object:	* + YSO (SIMBAD class: Star)
Note:	Himalayan Chandra 2m telescope (HCT, India) HFOSC observations of N=5 stars and N=111 YSOs in the field of the Planck cold clump PGCC G108.37-01.06. Use of archival CFHT WIRCam and Spitzer IRAC data.
in source:	PGCC G108.37-01.06
Ref:	=2018ApJ...864..154D
by	DUTTA S. , MONDAL S., SAMAL M.R., JOSE J.
	Astrophys. J., 864, 154-154 (2018)
	The Planck cold clump G108.37-01.06: a site of complex interplay between H II regions, young clusters, and filaments.
o	Fig. 3, Table 1: <[DMS2018] SNN> (Nos S01-S05). Table 3: <[DMS2018] JDDD.ddddd+DD.ddddd> N=111.
o	Figure 13: Filaments F1-F4 are not in SIMBAD.
=E=	Catalogue in electronic form as <J/ApJ/864/154/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMS2020]
[DMS2020]	(Da Silva+Menezes+Steiner, 2020)
Write:	<<[DMS2020] NN>> <<[DMS2020] NN>> <<[DMS2020] VN>>
N:	2+10+2
Object:	Part of G + HII + Optical Variable Source (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Gemini-South GMOS, SOAR SIFS observations of N=2 stellar nuclei (format NN), N=10 HII regions (format NN), and N=2 variable sources (format VN) in the nuclear region of NGC 613. Use of archival HST WFPC2, VLT SINFONI, Chandra ACIS, and ALMA data.
in source:	NGC 613
Ref:	=2020MNRAS.492.5121D
by	DA SILVA P. , MENEZES R.B., STEINER J.E.
	Mon. Not. R. Astron. Soc., 492, 5121-5140 (2020)
	The nuclear region of NGC 613 - I. Multiwavelength analysis.
o	Fig. 5, Tables 1-3: <[DMS2020] NN> (Nos N1-N2). Fig. 10, Tables 2-3: <[DMS2020] NN> (Nos 1-10). Figs 8-9: <[DMS2020] VN> (Nos V1-V2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMS93]
[DMS93]	(Drissen+Moffat+Shara, 1993)
Write:	<<[DMS93] NGC 595 NNN>> <<[DMS93] NGC 604 NNN>>
N:	113+207
Object:	* (SIMBAD class: Star)
in source:	M 33:NGC 595 = NGC 595
in source:	M 33:NGC 604 = NGC 604
Ref:	=1993AJ....105.1400D
by	DRISSEN L. , MOFFAT A.F.J., SHARA M.M.
	Astron. J., 105, 1400-1410 (1993)
	A Hubble Space Telescope planetary camera view of giant HII regions: the Wolf-Rayet content of NGC 595 and NGC 604 in M 33.
o	Table 1, col. (1): <[DMS93] NGC 595 NNN> N=113 among 121. Table 1, col. (WR?): <DMS NGC 595 NNa> (Nos 2a, 2b) added. Table 2, col (1): <[DMS93] NGC 604 NNN> N=207 among 254. Table 2, col. (WR?): <DMS NGC 604 NNa> (Nos 2a, 2b, 4a, 4b) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMS97]
[DMS97]	(Dalton+Maddox+Sutherland+, 1997)
*****	Avoid the usage of [DMS97], prefer APMCC
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMV2000]
[DMV2000]	(Donahue+Mack+Voit+, 2000) (Not yet in Simbad)
Write:	<<[DMV2000] ACO 2597 NN>> <<[DMV2000] PKS 0745-191 NN>>
N:	10+13
Object:	Clump (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=10 Clumps in ACO 2597. N=13 Clumps in PKS 0745-191.
in source:	ACO 2597
in source:	PKS 0745-191
Ref:	=2000ApJ...545..670D
by	DONAHUE M. , MACK J., VOIT G.M., SPARKS W., ELSTON R., MALONEY P.R.
	Astrophys. J., 545, 670-694 (2000)
	Hubble space telescope observations of vibrationally excited molecular hydrogen in cluster cooling flow nebulae.
o	Table 5, Fig.6: <[DMV2000] ACO 2597 NN> (Nos 1-10). Table 6: <[DMV2000] PKS 0745-191 NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMV2002]
[DMV2002]	(Di Carlo+Massi+Valentini+, 2002)
Write:	<<[DMV2002] N>> <<[DMV2002] CN>>
N:	9+3
Object:	* (SIMBAD class: Star)
Note:	Observations of SN 1999E1. N=9 local standards (Nos 1-9) and N=3 foreground stars near SN 1999EL (Nos C1-C3).
Ref:	=2002ApJ...573..144D
by	DI CARLO E. , MASSI F., VALENTINI G., DI PAOLA A., D'ALESSIO F., BROCATO E., GUIDUBALDI D., DOLCI M., PEDICHINI F., SPEZIALI R., LI CAUSI G., CARATTI O GARATTI A., CAPPELLARO E., TURATTO M., ARKHAROV A.A., GNEDIN Y., LARIONOV V.M., BENETTI S., PASTORELLO A., ARETXAGA I., CHAVUSHYAN V., VEGA O., DANZIGER I.J., TORNAMBE A.
	Astrophys. J., 573, 144-156 (2002)
	Optical and infrared observations of the supernova SN 1999el.
o	Fig.1, text: <[DMV2002] N> (Nos 1-9), <[DMV2002] CN> (Nos C1-C3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMW2013]
[DMW2013]	(DAWSON+McCLURE-GRIFFITHS+WONG+, 2013)
Write:	<<[DMW2013] NN>>
N:	11 (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Supergiant shells of atomic gas in the LMC from ATCA 21cm line observations.
in source:	NAME LMC
Ref:	=2013ApJ...763...56D
by	DAWSON J.R. , McCLURE-GRIFFITHS N.M., WONG T., DICKEY J.M., HUGHES A., FUKUI Y., KAWAMURA A.
	Astrophys. J., 763, 56 (2013)
	Supergiant shells and molecular cloud formation in the Large Magellanic Cloud.
o	Table 1: <[DMW2013] NN> (Nos 1-11)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMW95]
[DMW95]	(Dent+Matthews+Walther, 1995)
Write:	<<[DMW95] HN>>
N:	8
Object:	H2 Knot (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	JCMT observations. H2 knots in the field of AMDM VLA 1623.4-2418. See also AMDM.
in source:	AMDM VLA 1623.0-2418
Ref:	=1995MNRAS.277..193D
by	DENT W.R.F. , MATTHEWS H.E., WALTHER D.M.
	Mon. Not. R. Astron. Soc., 277, 193-209 (1995)
	CO and shocked H2 in the highly collimated outflow from VLA 1623.
o	Text: <AMDM Blue N> (No. 4) added. Fig.6, Table 2: <[DMW95] AN> (Nos H1-H8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMY2004]
[DMY2004]	(Dunlop+McLure+Yamada+, 2004)
Write:	<<[DMY2004] HDF 850.1K>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Note:	The authors identified the galaxy counterpart of the smm source [HSD98] HDF850.1 as 'HDF 850.1K'. See [HSD98]
Ref:	=2004MNRAS.350..769D
by	DUNLOP J.S. , McLURE R.J., YAMADA T., KAJISAWA M., PEACOCK J.A., MANN R.G., HUGHES D.H., ARETXAGA I., MUXLOW T.W.B., RICHARDS A.M.S., DICKINSON M., IVISON R.J., SMITH G.P., SMAIL I., SERJEANT S., ALMAINI O., LAWRENCE A.
	Mon. Not. R. Astron. Soc., 350, 769-784 (2004)
	Discovery of the galaxy counterpart of HDF 850.1, the brightest submillimetre source in the Hubble Deep Field.
o	HDF 850.1 = [HSD98] HDF850.1
o	<[DMY2004] HDF 850.1K> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DMZ2008]
[DMZ2008]	(De Luca+Mignani+Zaggia+, 2008) (Not yet in Simbad)
Write:	<<[DMZ2008] N>>
N:	7
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Archival VLT ISAAC and HST NICMOS IR observations. N=7 candidate counterparts of RCW 103.
Ref:	=2008ApJ...682.1185D
by	DE LUCA A. , MIGNANI R.P., ZAGGIA S., BECCARI G., MEREGHETTI S., CARAVEO P.A., BIGNAMI G.F.
	Astrophys. J., 682, 1185-1194 (2008)
	Deep infrared observations of the puzzling central X-ray source in RCW 103.
o	Fig.1, Table 4: <[DMZ2008] N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DN
DN	(Duus+Newell)
*****	Avoid the usage of DN, prefer Str
Details on Acronym: [DNB2016]
[DNB2016]	(De La Fuente+Najarro+Borissova+, 2016)
Write:	<<[DNB2016] Mc30-NNa>>
N:	24
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT ISAAC spectroscopic observations of N=24 stars in the field of Mercer 30.
in source:	NAME Mercer 30
Ref:	=2016A&A...589A..69D
by	DE LA FUENTE D. , NAJARRO F., BORISSOVA J., RAMIREZ ALEGRIA S., HANSON M.M., TROMBLEY C., FIGER D.F., DAVIES B., GARCIA M., KURTEV R., URBANEJA M.A., SMITH L.C., LUCAS P.W., HERRERO A.
	Astron. Astrophys., 589A, 69-69 (2016)
	Probing the Dragonfish star-forming complex: the ionizing population of the young massive cluster Mercer 30.
o	Table 2: <[DNB2016] Mc30-NNa> (Nos 1-24).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DNB89]
[DNB89]	(Diamond+Norris+Baan+, 1989)= (OH)
Write:	<<[DNB89] OH R>> <<[DNB89] OH IIa>>
N:	2+2
Object:	Maser component (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	OH Maser components I and II, with subcomponents IIa and IIb, in IC 4553 (APG 220)
in source:	APG 220 = IC 4553
Ref:	=1989ApJ...340L..49D
by	DIAMOND P.J. , NORRIS R.P., BAAN W.A., BOOTH R.S.
	Astrophys. J., 340, 49-52 (1989)
	VLBI observations of the OH megamaser in IC 4553 (Arp 220).
o	Table 1: <[DNB89] OH I>, <[DNB89] OH II>, <[DNB89] OH IIa>, <[DNB89] OH IIb>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DNCG
DNCG	(Duus+Newell, Cluster of G)
*****	Avoid the usage of DNCG, prefer Str
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [DNG99]
[DNG99]	(De Pree+Nysewander+Goss, 1999)
Write:	<<[DNG99] NGC 3603 A>>
N:	13
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA observations. Fig.2: 3.4cm continuum image of NGC 3603: N=13 sources (Nos A-M).
in source:	NGC 3603
Ref:	=1999AJ....117.2902D
by	DE PREE C.G. , NYSEWANDER M.C., GOSS W.M.
	Astron. J., 117, 2902-2918 (1999)
	NGC 3576 and NGC 3603: two luminous southern H II regions observed at high resolution with the Australia Telescope Compact Array.
o	IRS in Fig.1 = [FP74] RCW 57 IRS NN, IRS in Fig.2 = [FPA77] NGC 3603 IRS NN.
o	Table 2: <[DNG99] NGC 3603 A> (Nos A-M).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DNJ95]
[DNJ95]	(Doyon+Nadeau+Joseph+, 1995)
Write:	<<[DNJ95] A>>
N:	4
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
in source:	VV 114
Ref:	=1995ApJ...450..111D
by	DOYON R. , NADEAU D., JOSEPH R.D., GOLDADER J.D., SANDERS D.B., ROWLANDS N.
	Astrophys. J., 450, 111-121 (1995)
	Near-infrared imaging and spectroscopy of the bright IRAS galaxy VV 114.
o	Table 1: <[DNJ95] A> (Nos A-D)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DNM2003]
[DNM2003]	(De Breuck+Neri+Morganti+, 2003)
Write:	<<[DNM2003] J2330+3927 a>> <<[DNM2003] J2330+3927 Star>> <<[DNM2003] J2330+3927 CO>> <<[DNM2003] J2330+3927 W>>
N:	3+1+1+3
Object:	Part of G + (Rad) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Multi-frequency study of the radio galaxy B3 2327+391. N=3 components (Nos a-c), N=1 Offset star in the field, N=1 CO peak, and N=3 radio components (Nos N, C, S). [DNM2003] J2330+3927 a is the most likely AGN position from optical/IR observations but it is not coincident with the central radio component. See also [PD2005]
in source:	B3 2327+391
Ref:	=2003A&A...401..911D
by	DE BREUCK C. , NERI R., MORGANTI R., OMONT A., ROCCA-VOLMERANGE B., STERN D., REULAND M., VAN BREUGEL W., ROETTGERING H., STANFORD S.A., SPINRAD H., VIGOTTI M., WRIGHT M.
	Astron. Astrophys., 401, 911-925 (2003)
	CO emission and associated H I absorption from a massive gas reservoir surrounding the z = 3 radio galaxy B3 J2330+3927.
o	B3 J2330+3927 = B3 2327+391 in SIMBAD. 6C J1908+7220 (2000 coord.) = 6C 1909+7215 in SIMBAD. 8C 1425+635 is a misprint for 8C 1435+633. B3 J2330+3929 and J2330+3926 are misprint for B3 J2330+3927.
o	Fig.2, Table 1: <[DNM2003] J2330+3927 a> (Nos a-c), <[DNM2003] J2330+3927 Star> N=1, <[DNM2003] J2330+3927 CO> N=1. Table 3: <[DNM2003] J2330+3927 W> (Nos N, C, S).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DNS
DNS	(Deep Near-infrared Survey)
*****	Avoid the usage of DNS, prefer DENIS-P
Origin	of the Acronym: L (2001ApJ...548..908L)
Details on Acronym: [DNT2015]
[DNT2015]	(De La Fuente D.+Najarro F.+Trombley+, 2015)
Write:	<<[DNT2015] McNN-NN>>
N:	17+14
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT ISAAC medium-resolution spectroscopy and HST NICMOS photometry of N=17+14 stars ub the field of the young massive clusters Mercer 20 and Mercer 70.
in source:	[MCM2005b] 20
in source:	[MCM2005b] 70
Ref:	=2015A&A...575A..10D
by	DE LA FUENTE D. , NAJARRO F., TROMBLEY C., DAVIES B., FIGER D.F.
	Astron. Astrophys., 575A, 10-10 (2015)
	First detections of FS Canis Majoris stars in clusters. Evolutionary state as constrained by coeval massive stars.
o	Figs 7-8: <[DNT2015] McNN-NN> (Nos Mc20-1 to Mc20-17, Mc70-1 to Mc70-14). Table 4: <[DCT2012] DN-NN> (Nos D1-13, D1-14) added. Fig. 15, Table 4: <[DDN2012] NN> (No. 28) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DNZ2000]
[DNZ2000]	(Deharveng+Nadeau+Zavagno+, 2000)= (DNZC)
Write:	<<[DNZ2000] NNN>>
N:	125
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Star in Sh 2-88B region.
in source:	SH 2-88 B
Ref:	=2000A&A...360.1107D
by	DEHARVENG L. , NADEAU D., ZAVAGNO A., CAPLAN J.
	Astron. Astrophys., 360, 1107-1116 (2000)
	The stellar content of the compact HII region Sh2-88B.
o	Table 1: <[DNZ2000] NNN> (Nos 1-125).
=E=	Catalogue in electronic form as J/A+A/360/1107
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DNZ2010]
[DNZ2010]	(Deguchi+Nakashima+Zhang+, 2010)
Write:	<<[DNZ2010] McNN-N>> <<[DNZ2010] St2-NN>>
N:	18+18
Object:	Poss. Red Supergiant (SIMBAD class: RedSG_Candidate = Red Supergiant Candidate)
Note:	Nobeyama 45m radio telescope observations of red supergiant candidates in star clusters.
in source:	[MCM2005b] 4
in source:	[MCM2005b] 8
in source:	[MCM2005b] 13
in source:	Cl Stephenson 2
Ref:	=2010PASJ...62..391D
by	DEGUCHI S. , NAKASHIMA J., ZHANG Y., CHONG S.S.N., KOIKE K., KWOK S.
	PASJ, 62, 391-407 (2010)
	SiO and H2O maser observations of red supergiants in star clusters embedded in the Galactic disk.
o	Fig. 1, Table 1: <[DNZ2010] McNN-N> (Nos Mc4-1 to Mc4-5, Mc4-8, Mc8-1 to Mc8-6, Mc13-1 to Mc13-6), <[DNZ2010] St2-NN> N=18 among (Nos St2-01 to St2-29).
=E=	Catalogue in electronic form as J/PASJ/62/391
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DNZC
DNZC	(Deharveng+Nadeau+Zavagno+Caplan)
*****	Avoid the usage of DNZC, prefer [DNZ2000]
Origin	of the Acronym: L (2003ApJ...599.1173G)
Details on Acronym: DO
DO	(Dearborn Obs.)= (DB) = (DC)
Write:	<<DO NNNNN>>
N:	44076
Object:	Faint Red * (SIMBAD class: Star)
Note:	Part 1A: (Nos 1-8151), later re-named DC. Part 1B: (Nos 8141-22680), Stars numbered 8141-8151 in part 1A are identically repeated in part 1B. Part 1C: (Nos 22681-44076).
Ref:	=1947AnDea...5....1L
by	LEE O.J. , BALDWIN R.J., HAMLIN D.W., BARTLETT T.J., GORE G.D., BALDWIN T.J.
	Ann. Dearborn Obs., 5, 1-None (1947)
	Dearborn Observatory Catalogue of faint red stars (parts 1A, 1B and 1C).
o	Part IA: <DO NNNN> (Nos 1-8151). Part IB: <DO NNNNN> (Nos 8141-22680). Part IC: <DO NNNNN> (Nos 22681-44076).
=E=	Catalogue in electronic form as II/68
Details on Acronym: Do
Do	(Dolidze)
*****	Avoid the usage of Do, prefer Dd
Details on Acronym: Do-Ar
Do-Ar	(Dolidze+Arakelian)
*****	Avoid the usage of Do-Ar, prefer DoAr
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [DO2013]
[DO2013]	(Dewangan+Ojha, 2013)
Write:	<<[DO2013] sNN>> <<[DO2013] N>>
N:	39+8
Object:	YSO + * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Multi-wavelength analysis of N=39 YSOs and N=8 O-type star candidates around the mid-infrared bubble [CPA2006] N14. Use of UKIDSS Galactic Plane Survey, Spitzer GLIMPSE and MIPSGAL data.
in source:	[CPA2006] N14
Ref:	=2013MNRAS.429.1386D
by	DEWANGAN L.K. , OJHA D.K.
	Mon. Not. R. Astron. Soc., 429, 1386-1397 (2013)
	Multi-wavelength study of triggered star formation around the mid-infrared bubble N14.
o	Fig. 6, Table 1: <[DO2013] sNN> (Nos s1-s39). Fig. 7, Table 2: <[DO2013] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DO99]
[DO99]	(Dwarakanath+Owen, 1999)
Write:	<<[DO99] ACO NNNN NN>>
N:	54+36
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Search for optical identification of VLA detected cluster member candidates in 2 ACO clusters.
in source:	ACO 2125
in source:	ACO 2645
Ref:	=1999AJ....118..625D
by	DWARAKANATH K.S. , OWEN F.N.
	Astron. J., 118, 625-632 (1999)
	On the different radio source populations in the Butcher-Oemler clusters Abell 2125 and 2645.
o	Table 2: <[DO99] ACO 2125 NN> (Nos 1-54). Table 3: <[DO99] ACO 2645 NN> (Nos 1-36).
=E=	Catalogue in electronic form as J/AJ/118/625
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DOA2012]
[DOA2012]	(Dewangan+Ojha+Anandarao+, 2012)
Write:	<<[DOA2012] IRSN>>
N:	8 (SIMBAD class: YSO = Young Stellar Object)
Note:	Multi-wavelength observations around two bubbles associated with a southern massive star-forming region G8.14+0.23. Use of archival UKIDSS, 2MASS, and Spitzer GLIMPSE data.
in source:	GAL 008.14+00.23
Ref:	=2012ApJ...756..151D
by	DEWANGAN L.K. , OJHA D.K., ANANDARAO B.G., GHOSH S.K., CHAKRABORTI S.
	Astrophys. J., 756, 151 (2012)
	Triggered star formation around mid-infrared bubbles in the G8.14+0.23 H II region.
o	Table 1: <[DOA2012] IRSN> (Nos 1-8)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DoAr
DoAr	(Dolidze+Arakelian)= (Do-Ar)
Write:	<<DoAr NN>>
N:	88
Object:	Em* in Assoc. (SIMBAD class: EmLine* = Emission-line Star)
in source:	NAME rho Oph Cloud
Ref:	=1959AZh....36..444D
by	DOLIDZE M.V. , ARAKELIAN M.A.
	Astron. Zh., 36, 444-None (1959)
	The T-association near ρ Ophiuchi.
o	= 1959SvA.3.434D
o	Tables 1, 2: <DoAr NN> (Nos 1-88)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [DOB2000]
[DOB2000]	(De Grijs+O'Connell+Becker+, 2000)= ([DOB2000a])
Write:	<<[DOB2000] NN>>
N:	36
Object:	H-alpha source (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations. N=36 H-alpha sources in M 82, (Nos 1-10) are possible SNR.
in source:	M 82 = NGC 3034
Ref:	=2000AJ....119..681D
by	DE GRIJS R. , O'CONNELL R.W., BECKER G.D., CHEVALIER R.A., GALLAGHER III J.S.
	Astron. J., 119, 681-687 (2000)
	Supernova remnants in the fossil starburst in M82.
o	in ref list Braun, Goss, Lyne 1989ApJ...340..355B instead of 340.555
o	Text: <[OM78] AN> (Nos B1-B2) added. Table 1: <[DOB2000] NN> (Nos 1-36).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DOB2000a]
[DOB2000a]	(De Grijs+O'Connell+Becker+, 2000)
*****	Avoid the usage of [DOB2000a], prefer [DOB2000]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DOB2000b]
[DOB2000b]	(De Vries+O'Dea+Barthel+, 2000)
Write:	<<[DOB2000b] 3C 46b>> <<[DOB2000b] 0941-080b>> <<[DOB2000b] 3C 460b>>
N:	3
Object:	G (SIMBAD class: GinPair = Galaxy in Pair of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=3 interacting companion galaxies, principal galaxies: 3C 46, PKS 0941-080, 3C 460.
Ref:	=2000AJ....120.2300D
by	DE VRIES W.H. , O'DEA C.P., BARTHEL P.D., FANTI C., FANTI R., LEHNERT M.D.
	Astron. J., 120, 2300-2330 (2000)
	Hubble space telescope NICMOS observations of the host galaxies of powerful radio sources: does size matter?
o	Table 1: <[DOB2000b] 3C 46b> N=1, <[DOB2000b] 0941-080b> N=1, <[DOB20O0b] 3C 460b> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DOBASHI
DOBASHI	(DOBASHI)
Write:	<<DOBASHI NNNN>>
N:	7614
Object:	Dark Nebula (SIMBAD class: DarkNeb = Dark Cloud (nebula))
Stat:	is completely incorporated in Simbad
Note:	Survey for dark clouds based on the 2 MASS Point Source Catalog. N=7614 dark clouds mainly consisting of "dense cores".
Notes:	The list of the 7614 clouds and its byte-by-byte description can be found at the following URL: http://darkclouds.u-gakugei.ac.jp/2MASS/cloud_list.txt http://darkclouds.u-gakugei.ac.jp/more/readme2mass.html
Ref:	=2011PASJ...63S...1D
by	DOBASHI K.
	PASJ, 63S, 1-362 (2011)
	Atlas and Catalog of Dark Clouds Based on the 2 Micron All Sky Survey.
o	Table 8: <DOBASHI NNNN> (Nos 1-7614).
=E=	Catalogue in electronic form as <J/PASJ/63/S1/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: DOC
DOC	(Deep Optical Catalog)= (MGBR)
Write:	<<DOC SRGaNNN>> <<DOC NRGaNNN>> <<DOC SRGaNNN.NN>> <<DOC NRGaNNN.NN>>
N:	20+877
Object:	Group of G + G in Group (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=20 groups of galaxies. In the format 'SRG' and 'NRG' stand for Southern CfA and Northern CfA. Table 2: N=907 galaxies in the groups. Preliminary catalogue. See also finalcatalogue RASSCALS.
Ref:	=1999ApJ...518...69M
by	MAHDAVI A. , GELLER M.J., BOHRINGER H., KURTZ M.J., RAMELLA M.
	Astrophys. J., 518, 69-93 (1999)
	The dynamics of poor systems of galaxies.
o	Table 1: <DOC SRGaNNN>, <DOC NRGaNNN>, N=20. Table 2: <DOC SRGaNNN.NN>, <DOC NRGaNNN.NN>, N=877.
=E=	Catalogue in electronic form as J/ApJ/518/69
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DOC05
DOC05	(De Buizer+Osorio+Calvet, 2005)
*****	Avoid the usage of DOC05, prefer [DRT2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DoDz
DoDz	(Dolidze+Dzimselejsvili)
*****	Avoid the usage of DoDz, prefer Dolidze-Dzim
Origin	of the Acronym: L (2001A&A...366..827B)
Details on Acronym: DoDz
DoDz	(Dolidze+Dzimselejsvili)
*****	Avoid the usage of DoDz, prefer DdDm
Details on Acronym: DOG
DOG	(Dust Obscured Galaxy)
*****	Avoid the usage of DOG, prefer [BDL2009]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DOG
DOG	(Dust Obscured Galaxy)
*****	Avoid the usage of DOG, prefer [MDA2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DOG2001]
[DOG2001]	(De Grijs+O'Connell+Gallagher, 2001)
Write:	<<[DOG2001] B1 NN>> <<[DOG2001] B2 NN>>
N:	43+70
Object:	Poss. Stellar Cluster (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 and NICMOS imaging of the regions [OM78] B1 and B2 in the galaxy M 82. Tables 2 and 3: stellar cluster candidates samples.
in source:	M 82 = NGC 3034
Ref:	=2001AJ....121..768D
by	DE GRIJS R. , O'CONNELL R.W., GALLAGHER III J.S.
	Astron. J., 121, 768-792 (2001)
	The fossil starburst in M82.
o	Table 2: <[DOG2001] B1 NN> (Nos 1-43). Table 3: <[DOG2001] B2 NN> (Nos 1-70).
=E=	Catalogue in electronic form as J/AJ/121/768
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DOG93]
[DOG93]	(Dressler+Oemler+Gunn+, 1993)
Write:	<<[DOG93] A>> <<[DOG93] N>>
N:	8+8
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Plate L6, Fig. 5: format 'A', (Nos A-H), probable members of the foreground cluster C 0939+4713 format 'N', (Nos 1-8), possible members of the foreground cluster C 0939+4713
in source:	NAME C 0939+4713
Ref:	=1993ApJ...404L..45D
by	DRESSLER A. , OEMLER A., GUNN J.E., BUTCHER H.
	Astrophys. J., 404, 45-49 (1993)
	A cluster of nascent galaxies at z = 2 ?
o	Object Q in fig. 2, described p. L46, is [DG92] 4-440 in Simbad
o	Plate L6, Fig. 5: <[DOG93] A> (Nos A-H), <[DOG93] N> N=8
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DOH
DOH	(Doi+O'Dell+Hartigan)
Write:	<<DOH NN>> <<DOH NN SSs-MSS>>
N:	15+72
Object:	Feature (SIMBAD class: HerbigHaroObj = Herbig-Haro Object)
Note:	HST WFPC2 observations The [OW94] features are physically associated with HH objects, or are forming 15 new groups 'DOH NN' of features or knots, designated as 'DOH NN SSs-MSS'. See also [OW94].
in source:	NAME Orion Nebula
Ref:	=2004AJ....127.3456D
by	DOI T. , O'DELL C.R., HARTIGAN P.
	Astron. J., 127, 3456-3478 (2004)
	Internal velocities in the Orion nebula: large radial velocity features.
o	Table 1: complete coord. of 'SSs-MSS' are J2000: 05 35 SS.s -05 2M SS.
o	Table 1, first part: <[OW94] SSs-MMS> N=57. Table 1, second part: <[OW94] SSs-MSS> = <DOH NN SSs-MSS> N=72. Text: <DOH NN> (Nos 1-15).
=E=	Catalogue in electronic form as J/AJ/127/3456
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DoH
DoH	(Dobashi, High-resolution)
*****	Avoid the usage of DoH, prefer TGU
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: Doi
Doi	(Doi+)
*****	Avoid the usage of Doi, prefer [DFO95]
Origin	of the Acronym: L (2001AJ....121..683H)
Details on Acronym: Dolidze
Dolidze	(Dolidze)
Write:	<<Cl Dolidze NN>>
N:	47
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Note:	ref. 1961ACiCh.223...11D: (Nos 1-15). The numbering is continued in different russian references, till number 47 (but a Cl Dolidze 78 is found in ref. 1996A&A...305..457M)
Ref:	=1961ACiCh.223...11D
by	DOLIDZE M.V.
	Astron. Cir., 223, 11-12 (1961)
	On the star cluster near γ Cyg.
o	Tables 1, 2: <Cl Dolidze NN> (Nos 1-15)
Details on Acronym: Dolidze
Dolidze	(Dolidze+)
*****	Avoid the usage of Dolidze, prefer [DV59]
Origin	of the Acronym: L (1996Ap.....39...27M)
Details on Acronym: Dolidze-Dzim
Dolidze-Dzim	(Dolidze+Dzimselejsvili)= (DoDz)
Write:	<<Cl Dolidze-Dzim NN>>
N:	11
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Ref:	=1966ATsir.382....7D
by	DOLIDZE M.V. , JIMSHELEISHVILI G.N.
	ATsir, 382, 7-8 (1966)
	New possible star clusters.
o	Table: <Cl Dolidze-Dzim NN> (Nos 1-11).
Details on Acronym: Don
Don	(Discoverer's name: Donner)
Write:	<<** DON NNNN>>
N:	1031
Object:	(SIMBAD class: = Double or Multiple Star)
Ref:	=1955POMic..11....1R
by	ROSSITER R.A.
	Publ. Michigan Obs., 11, 1-None (1955)
	Catalogue of southern double stars.
o	Catalogue: < Don NNNN> N=1031 among (Nos 1-1057). < Jsp NNN> N=803 among (Nos 1-854). < RDS NNNN> (Nos 1-8065). < Rst NNNN> N=5534 among (Nos 1-5560).
Details on Acronym: [DOP2013]
[DOP2013]	(Dressler+Oemler+Poggianti+, 2013)
Write:	<<[DOP2013] RCSHHMMA>> <<[DOP2013] SDSSHHMMA>> <<[DOP2013] RCSHHMMA-NA>> <<[DOP2013] SDSSHHMMA-NA>> <<[DOP2013] RCSHHMM NNA>> <<[DOP2013] SDSSHHMM NA>>
Object:	Cluster of G + Group of G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Identification of group of galaxies in N=5 rich clusters and the field at 0.31<z<0.54. Use of IMACS Cluster Building Survey (ICBS).
Ref:	=2013ApJ...770...62D
by	DRESSLER A. , OEMLER A.Jr, POGGIANTI B.M., GLADDERS M.D., ABRAMSON L., VULCANI B.
	Astrophys. J., 770, 62 (2013)
	The IMACS cluster building survey. II. Spectral evolution of galaxies in the epoch of cluster assembly.
o	Sources in table 7 are not in Simbad.
o	Table 1: <[DOP2013] RCSHHMMA> (Nos RCS0221A and RCS1102B), <[DOP2013] SDSSHHMMA> N=3. Table 4: <[DOP2013] RCS0221A-NA> N=5, <[DOP2013] RCS1102B-NA> N=6, <[DOP2013] SDSS0845A-N> (Nos 1-2), <[DOP2013] SDSS1500A-NA> N=5, <[DOP2013] SDSS1500B-NA> N=6. Table 5: <[DOP2013] RCS0221 NA> N=9, <[DOP2013] RCS1102 NN N=7 among (Nos 1-10), <[DOP2013] SDSS0845 NA> N=3, <[DOP2013] SDSS1500 N> N=4. Table 6: <[DOP2013] RCS1102 N> N=3, <[DOP2013] SDSS0845 NA> N=2, <[DOP2013] SDSS1500 N> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DOP2016]
[DOP2016]	(Dunham+Offner+Pineda+, 2016) (Not yet in Simbad)
Write:	<<[DOP2016] CHAI-NN>> <<[DOP2016] CHAI-NN-A>>
N:	24
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	ALMA Band 3 (106GHz) observations of N=24 continuum sources in 19 target fields in the Chamaeleon I molecular cloud.
in source:	NAME Cha I
Ref:	=2016ApJ...823..160D
by	DUNHAM M.M. , OFFNER S.S.R., PINEDA J.E., BOURKE T.L., TOBIN J.J., ARCE H.G., CHEN X., DI FRANCESCO J., JOHNSTONE D., LEE K.I., MYERS P.C., PRICE D., SADAVOY S.I., SCHNEE S.
	Astrophys. J., 823, 160 (2016)
	An ALMA search for substructure, fragmentation, and hidden protostars in starless cores in Chamaeleon I.
o	Table 4: Sources SSTgb are not in SIMBAD and 2MASS J11063460-7723340 was not identified.
o	Table 2: <[DOP2016] CHAI-NN-A> N=24 among (Nos 01-77).
=E=	Catalogue in electronic form as <J/ApJ/823/160/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Dor
Dor	(Doradus, InfraRed Source)= (H) = (HSJG) = (IRS)
Write:	<<Dor IRS NNN>>
N:	175
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Infrared survey of Dor Nebula complex. Identif. charts See also [HSJ92].
in source:	Magellanic Clouds:LMC:30 Dor Nebula = 30 Dor Nebula
Ref:	=1992MNRAS.257..391H
by	HYLAND A.R. , STRAW S., JONES T.J., GATLEY I.
	Mon. Not. R. Astron. Soc., 257, 391-403 (1992)
	Star formation in the Magellanic Clouds. IV. Protostars in the vicinity of 30 Doradus.
o	Table 2: <Dor IRS NNN> (Nos 1-175). Table 3: <[HSJ92] PN> (Nos P1-P4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Dor IR
Dor IR	(Doradus, IR)
*****	Avoid the usage of Dor IR, prefer MH
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 30Dor-NIC
30Dor-NIC	(30 Dor nebula, NICMOS)
Write:	<<30Dor-NIC NNa>>
N:	24
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	HST NICMOS observation of the 30 Dor Nebula. N=24 sources with NIR excess, format 'NNa'. See also [BGB2001].
in source:	Magellanic Clouds:LMC:30 Dor Nebula = 30 Dor Nebula
Ref:	=2001AJ....122..858B
by	BRANDNER W. , GREBEL E.K., BARBA R.H., WALBORN N.R., MONETI A.
	Astron. J., 122, 858-865 (2001)
	Hubble space telescope NICMOS detection of a partially embedded, intermediate-mass, pre-main-sequence population in the 30 Doradus nebula.
o	Table 3: 'Knot N' = '[WB87] N'. In Table 2, IRSN-134 is a misprint for IRSN-137 (cf. 2013AJ....145...98W).
o	Tables 1, 2: <30Dor-NIC NNa> N=24. Table 3: <[BGB2001] Naa> N=8.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Dow
Dow	(Downes)= (Downes) (Not yet in Simbad)
Write:	<<Dow NNN>>
N:	117
Object:	SNR (SIMBAD class: SNRemnant = SuperNova Remnant)
Ref:	=1971AJ.....76..305D
by	DOWNES D.
	Astron. J., 76, 305-316 (1971)
	New radio results on supernova remnants.
o	Table I not in SIMBAD
o	Table I: <Dow NNN> (Nos 1-117)
Origin	of the Acronym: L (1974Ap&SS..27....3M)
Details on Acronym: Downes
Downes	(Downes) (Not yet in Simbad)
*****	Avoid the usage of Downes, prefer Dow
Origin	of the Acronym: L = Found in the literature
Details on Acronym: DP
DP	(De Marchi+Paresce)
Write:	<<DP N>>
N:	4
Object:	Poss. Catacl. V* (SIMBAD class: CataclyV* = Cataclysmic Binary)
Stat:	is completely incorporated in Simbad
Note:	HST FOC observations
in source:	NGC 6397
Ref:	=1994A&A...281L..13D
by	DE MARCHI G. , PARESCE F.
	Astron. Astrophys., 281, 13-16 (1994)
	Faint blue stars in the core of NGC 6397.
o	<DP N> N=4
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DP
DP	(Dolidze+Ponomareva)
*****	Avoid the usage of DP, prefer [DP65]
Origin	of the Acronym: L (1999A&AS..134..255K)
Details on Acronym: DP
DP	(D. Peton-Jonas)= (DP)
*****	Avoid the usage of DP, prefer [P81]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DP65]
[DP65]	(Dolidze+Ponomareva, 1965)= (DP)
Write:	<<[DP65] NN>>
N:	65
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Ref:	=1965SvA.....9..157D
by	DOLIDZE M.V. , PONOMAREVA G.A.
	Sov. Astron., 9, 157-None (1965)
	New emission stars in Cas.
o	Table 2: <[DP65] NN> (Nos 1-65).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DP70]
[DP70]	(Drilling+Philip, 1970)
Write:	<<[DP70] NNN>>
N:	113
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Early-type stars in the region 3HLF4. Data used in 1971AJ.....76.1072D. See also [P67], PS, [PD70], [D73].
Ref:	=1970BOTT....5..307D
by	DRILLING J.S. , PHILIP A.G.D.
	Bol. Obs. Tonantz. Tacub., 5, 307-316 (1970)
	A finding list of stars of spectral type A7 and earlier in regions at high galactic latitudes. IV. 3HLF4.
o	Table 1: Numbering 'NN' not used in SIMBAD.
o	Table 2: <[DP70] NNN> (Nos 1-113).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DP83]
[DP83]	(De Pater+Perley, 1983)= (3C)
Write:	<<[DP83] 3C 279 ANNa>>
N:	24+9
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Components of 3C 279.
Ref:	=1983ApJ...273...64D
by	DE PATER I. , PERLEY R.A.
	Astrophys. J., 273, 64-69 (1983)
	The radio structure of 3C 279.
o	Figs 1-4: <[DP83] 3C 279 A> (Nos A-G).
Ref:	=1989ApJ...340..117U
by	UNWIN S.C. , COHEN M.H., BIRETTA J.A., HODGES M.W., ZENSUS J.A.
	Astrophys. J., 340, 117-128 (1989)
	Superluminal motion in the quasar 3C 279.
o	Fig.1: <[DP83] 3C 279 AN> (Nos C1-C4) added.
Ref:	=1995AJ....110.2479L
by	LEPPANEN K.J. , ZENSUS J.A.
	Astron. J., 110, 2479-2492 (1995)
	Linear polarization imaging with very long baseline interferometry at high frequencies.
o	<[PUC81] 3C 273 AN> (Nos F1-F7) added. <[DP83] 3C 279 AN> (Nos C5-C7) added. <[UCP83] 3C 345 AN> (Nos C7-C8) added.
Ref:	=1998ApJ...504..702L
by	LISTER M.L. , MARSCHER A.P., GEAR W.K.
	Astrophys. J., 504, 702-719 (1998)
	Submilliarcsecond polarimetric imaging of blazer jets at 43 GHz.
o	Table 2: 1055+081 is a misprint for QSO 1055+018
o	Table 2: <[LMG98] HHMM+DDd A> N=8, <[LMG98] HHMM+DDd CN> N=4+2+3+2+5. Table 2: <[KWG93] OJ287 CN> (Nos C3-C6) added. Table 2: <[PK97] 1611+343 CNa> (Nos C5a, C6, C7) added. Table 2: <[DP83] 3C 279 CN> (No. C8) added.
Ref:	=2001ApJS..133..297W
by	WEHRLE A.E. , PINER B.G., UNWIN S.C., ZOOK A.C., XU W., MARSCHER A.P., TERASRANTA H., VALTAOJA E.
	Astrophys. J., Suppl. Ser., 133, 297-320 (2001)
	Kinematics of the parsec-scale relativistic jet in quasar 3C 279: 1991-1997.
o	Table 3: <[DP83] 3C 279 ANa> (Nos C9, C5a, C7a) added.
Ref:	=2004AJ....127.3115J
by	JORSTAD S.G. , MARSCHER A.P., LISTER M.L., STIRLING A.M., CAWTHORNE T.V., GOMEZ J.-L., GEAR W.K.
	Astron. J., 127, 3115-3120 (2004)
	Change in speed and direction of the jet near the core in the quasar 3C 279.
o	Table 2: <[DP83] 3C 279 ANN> (Nos C10-C16) added.
Ref:	=2008ApJ...689...79C
by	CHATTERJEE R. , JORSTAD S.G., MARSCHER A.P., OH H., McHARDY I.M., ALLER M.F., ALLER H.D., BALONEK T.J., MILLER H.R., RYLE W.T., TOSTI G., KURTANIDZE O., NIKOLASHVILI M., LARIONOV V.M., HAGEN-THORN V.A.
	Astrophys. J., 689, 79-94 (2008)
	Correlated multi-wave band variability in the blazar 3C 279 from 1996 to 2007.
o	Table 5: <[DP83] 3C 279 ANN> (Nos 17-23) added.
Ref:	=2008A&A...492..389L
by	LARIONOV V.M. , JORSTAD S.G., MARSCHER A.P., RAITERI C.M., VILLATA M., AGUDO I., ALLER M.F., ARKHAROV A.A., ASFANDIYAROV I.M., BACH U., BACHEV R., BERDYUGIN A., BOETTCHER M., BUEMI C.S., CALCIDESE P., CAROSATI D., CHARLOT P., CHEN W.-P., DI PAOLA A., DOLCI M., DOGRU S., DOROSHENKO V.T., EFIMOV Yu.S., ERDEM A., FRASCA A., FUHRMANN L., GIOMMI P., GLOWIENKA L., GUPTA A.C., GURWELL M.A., HAGEN-THORN V.A., HSIAO W.-S., IBRAHIMOV M.A., JORDAN B., KAMADA M., KONSTANTINOVA T.S., KOPATSKAYA E.N., KOVALEV Y.Y., KOVALEV Y.A., KURTANIDZE O.M., LAEHTEENMAEKI A., LANTERI L., LARIONOVA L.V., LETO P., LE CAMPION P., LEE C.-U., LINDFORS E., MARILLI E., McHARDY I., MINGALIEV M.G., NAZAROV S.V., NIEPPOLA E., NILSSON K., OHLERT J., PASANEN M., PORTER D., PURSIMO T., ROS J.A., SADAKANE K., SADUN A.C., SERGEEV S.G., SMITH N., STRIGACHEV A., SUMITOMO N., TAKALO L.O., TANAKA K., TRIGILIO C., UMANA G., UNGERECHTS H., VOLVACH A., YUAN W.
	Astron. Astrophys., 492, 389-400 (2008)
	Results of WEBT, VLBA and RXTE monitoring of 3C 279 during 2006-2007.
o	Text, Fig.6: <[DP83] 3C 279 ANN> (No. 24) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPB99]
[DPB99]	(Duc+Papaderos+Balkowski+, 1999)
Write:	<<[DPB99] HHHMM+DDMM>> <<[DPB99] HHHMM+DDMM GN>>
N:	20+7
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=20 HI dwarf galaxy candidates from a sample of HI sources in Hydra I Cluster. Text: 5 of the dwarf galaxy candidates have companions or nearby background galaxies, same format ending by 'GN'.
in source:	NAME Hya I Cluster
Ref:	=1999A&AS..136..539D
by	DUC P.-A. , PAPADEROS P., BALKOWSKI C., CAYATTE V., THUAN T.X., VAN DRIEL W.
	Astron. Astrophys., Suppl. Ser., 136, 539-569 (1999)
	HI-rich dwarf galaxies in the Hydra I cluster. I. Photometric and HI data.
o	Table 1: <[DPB99] AHHMM+DDMM> N=20. Text: <[DPB99] AHHMM+DDMM GN> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPC2015]
[DPC2015]	(De Cicco+Paolillo+Covone+, 2015)
Write:	<<[DPC2015] NN>>
N:	83
Object:	Poss. AGN (SIMBAD class: AGN_Candidate = Active Galaxy Nucleus Candidate)
Stat:	is completely incorporated in Simbad
Note:	VLT Survey Telescope (VST) observations of N=83 AGN candidates. Use of images from the SUpernova Diversity And Rate Evolution (SUDARE) survey.
in source:	NAME COSMOS Field
Ref:	=2015A&A...574A.112D
by	DE CICCO D. , PAOLILLO M., COVONE G., FALOCCO S., LONGO G., GRADO A., LIMATOLA L., BOTTICELLA M.T., PIGNATA G., CAPPELLARO E., VACCARI M., TREVESE D., VAGNETTI F., SALVATO M., RADOVICH M., BRANDT W.N., CAPACCIOLI M., NAPOLITANO N.R., SCHIPANI P.
	Astron. Astrophys., 574A, 112-112 (2015)
	Variability-selected active galactic nuclei in the VST-SUDARE/VOICE survey of the COSMOS field.
o	Table 3: <[DPC2015] NN> (Nos 1-83).
=E=	Catalogue in electronic form as J/A+A/574/A112
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPC99]
[DPC99]	(Desert+Puget+Clements, 1999)
Write:	<<[DPC99] HDF-N-LWN-NN>> <<[DPC99] HDF-ALL-LW3-NN>>
N:	4+2+18+15+23+41
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	ISO CAM observations. In the format 'LWN' stands for the LW field number. A few cross-identif. between the tables. See also ISOHDF, [ACE99], [GOS97].
in source:	NAME HDFN
Ref:	=1999A&A...342..363D
by	DESERT F.-X. , PUGET J.-L., CLEMENTS D.L., PERAULT M., ABERGEL A., BERNARD J.-P., CESARSKY C.J.
	Astron. Astrophys., 342, 363-377 (1999)
	A classical approach to faint extragalactic source extraction from ISOCAM deep surveys. Application to the Hubble Deep Field.
o	Tables 1 to 5: <[DPC99] HDF-N-LWN-NN> = <ISOHDF JHHMMSS.s+DDMMSS>, N=4+2+18+15+23. Table 6: <[DPC99] HDF-ALL-LW3-NN> = <ISOHDF JHHMMSS.s+DDMMSS> N=41.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPD2006]
[DPD2006]	(Dessauges-Zavadsky+Prochaska+D'Odorico+, 2006)
Write:	<<[DPD2006] QSO JHHMM+DDMM abs N.NNNNN>>
N:	17+10+7+7+23+4
Object:	Absorber
Note:	UVES/VLT spectra combined with existing HIRES/Keck spectra. See also Paper I: [DCP2004].
Ref:	=2006A&A...445...93D
by	DESSAUGES-ZAVADSKY M. , PROCHASKA J.X., D'ODORICO S., CALURA F., MATTEUCCI F.
	Astron. Astrophys., 445, 93-113 (2006)
	A new comprehensive set of elemental abundances in DLAs. II. Data analysis and chemical variation studies.
o	Tables 2-8: <[DPD2006] QSO JHHMM+DDMM abs N.NNNNN> N=17+10+7+7+23+4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPD83]
[DPD83]	(De Vaucouleurs+Pence+Davoust, 1983)= (deV)
Write:	<<[DPD83] NN>> <<[DPD83] A>>
N:	60+3
Object:	HII + * (SIMBAD class: HIIReg = HII Region)
Note:	Table 3: format 'NN', N=60 HII in M83. format 'A', N=3 * in M83.
in source:	M 83 = NGC 5236
Ref:	=1983ApJS...53...17D
by	DE VAUCOULEURS G. , PENCE W.D., DAVOUST E.
	Astrophys. J., Suppl. Ser., 53, 17-39 (1983)
	Velocity fields in late-type galaxies from Hα Fabry-Perot interferometry. IV. Kinematics and dynamics of the SAB(s)c spiral NGC 5236 (M 83).
o	<[DPD83] NN> N=60, <[DPD83] A> N=3
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPF2002]
[DPF2002]	(Duc+Poggianti+Fadda+, 2002)= ([DPF2002a])
Write:	<<[DPF2002] NN>> <<[DPF2002] JHHMMSS.ss+DDMMSS.s>>
N:	74+18
Object:	G (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	N=74 galaxies in ACO 1689, and N=18 foreground or background galaxies.
Ref:	=2002A&A...382...60D
by	DUC P.-A. , POGGIANTI B.M., FADDA D., ELBAZ D., FLORES H., CHANIAL P., FRANCESCHINI A., MOORWOOD A., CESARSKY C.
	Astron. Astrophys., 382, 60-83 (2002)
	Hidden star-formation in the cluster of galaxies Abell 1689.
o	Table 1: <[DPF2002] NN> (Nos 1-74). Table 4: <[DPF2002] JHHMMSS.ss+DDMMSS.s> N=18.
=E=	Catalogue in electronic form as J/A+A/382/60
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPF2002a]
[DPF2002a]	(Duc+Poggianti+Fadda+, 2002)
*****	Avoid the usage of [DPF2002a], prefer [DPF2002]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPF2002b]
[DPF2002b]	(D'Amico+Possenti+Fici+, 2002)
Write:	<<[DPF2002b] Psr A>>
N:	5
Object:	ms Psr (SIMBAD class: Pulsar)
Stat:	is completely incorporated in Simbad
Note:	N=5 millisecond pulsars in NGC 6752, also found repectivelely with an ID PSR: PSR J1911-5958A, PSR J1910-5959B, PSR J1911-6000C, PSR J1910-5959D, PSR J1910-5959E.
in source:	NGC 6752
Ref:	=2002ApJ...570L..89D
by	D'AMICO N. , POSSENTI A., FICI L., MANCHESTER R.N., LYNE A.G., CAMILO F., SARKISSIAN J.
	Astrophys. J., 570, 89-92 (2002)
	Timing of millisecond pulsars in NGC 6752: evidence for a high Mass-to-Light ratio in the cluster core.
o	Fig.1, Table 1: <[DPF2002b] Psr A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPF2010]
[DPF2010]	(D'Avanzo+Perri+Fugazza+, 2010)
Write:	<<[DPF2010] GRB 090205 Host G>>
N:	1
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS1 optical/NIR observations of GRB 090205 host galaxy.
Ref:	=2010A&A...522A..20D
by	D'AVANZO P. , PERRI M., FUGAZZA D., SALVATERRA R., CHINCARINI G., MARGUTTI R., WU X.F., THOENE C.C., FERNANDEZ-SOTO A., UKWATTA T.N., BURROWS D.N., GEHRELS N., MESZAROS P., TOMA K., ZHANG B., COVINO S., CAMPANA S., D'ELIA V., DELLA VALLE M., PIRANOMONTE S.
	Astron. Astrophys., 522A, 20-20 (2010)
	The afterglow and host galaxy of GRB 090205: evidence of a Ly-α emitter at z = 4.65.
o	<[DPF2010] GRB 090205 Host G> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPF2019]
[DPF2019]	(De Cicco+Paolillo+Falocco+, 2019)
Write:	<<[DPF2019] NNN>>
N:	299
Object:	Poss. AGN (SIMBAD class: AGN_Candidate = Active Galaxy Nucleus Candidate)
Stat:	is completely incorporated in Simbad
Note:	VLT Survey Telescope (VST) OmegaCAM observations of N=299 AGN candidates in the COSMOS field. See also [DPC2015].
in source:	NAME COSMOS Field
Ref:	=2019A&A...627A..33D
by	DE CICCO D. , PAOLILLO M., FALOCCO S., POULAIN M., BRANDT W.N., BAUER F.E., VAGNETTI F., LONGO G., GRADO A., RAGOSTA F., BOTTICELLA M.T., PIGNATA G., VACCARI M., RADOVICH M., SALVATO M., COVONE G., NAPOLITANO N.R., MARCHETTI L., SCHIPANI P.
	Astron. Astrophys., 627A, 33-33 (2019)
	Optically variable AGN in the three-year VST survey of the COSMOS field.
o	Table 3: <[DPF2019] NNN> (Nos 1-299).
=E=	Catalogue in electronic form as <J/A+A/627/A33/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPG2009]
[DPG2009]	(De La Fuente+Porras+Grave+, 2009)
Write:	<<[DPG2009] NN>>
N:	19
Object:	UC HII source (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	N=19 ultracompact (UC) HII sources in ultracompact HII regions with IRAC emission. Use of Spitzer IRAC data and VLA observations at 3.6cm.
Ref:	=2009RMxAC..37...13D
by	DE LA FUENTE E. , PORRAS A., GRAVE J.M.C., KUMAR M.S.N., TRINIDAD M.A., KURTZ S., KEMP S., FRANCO J., QUEVEDO G.
	RMxAC, 37, 13-20 (2009)
	Spitzer-IRAC imagery and photometry of ultracompact H II regions with extended emission.
o	Table 2: <[DPG2009] NN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPG99]
[DPG99]	(Drinkwater+Phillipps+Gregg+, 1999)
Write:	<<[DPG99] JHHMMSS.ss+DDMMSS.s>>
N:	13
Object:	Compact G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Fornax spectroscopic survey with 2dF on AAO telescope. Sample of 13 bright compact galaxies behind the Fornax Cluster.
Ref:	=1999ApJ...511L..97D
by	DRINKWATER M.J. , PHILLIPPS S., GREGG M.D., PARKER Q.A., SMITH R.M., DAVIES J.I., JONES J.B., SADLER E.M.
	Astrophys. J., 511, 97-100 (1999)
	The Fornax spectroscopic survey: the number of unresolved compact galaxies.
o	Table 1: <[DPG99] JHHMMSS.ss+DDMMSS.s> N=13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPK2003]
[DPK2003]	(Dessauges-Zavadsky+Peroux+Kim+, 2003)
Write:	<<[DPK2003] QSO JHHMM+DDMM abs N.NNN>> <<[DPK2003] QSO JHHMM+DDMM abs N.NNNNNN>>
N:	18+121
Object:	DLA
Note:	DLAs and sub-DLAs systems in QSOs. Some are already known with an other acronym.
Ref:	=2003MNRAS.345..447D
by	DESSAUGES-ZAVADSKY M. , PEROUX C., KIM T.-S., D'ODORICO S., McMAHON R.G.
	Mon. Not. R. Astron. Soc., 345, 447-479 (2003)
	A homogeneous sample of sub-damped Lyman α systems - I. Construction of the sample and chemical abundance measurements.
o	Tables 2 to 14: component structure of sub-DLA systems with z(abs) 'N.NNNNNN' are not in SIMBAD.
o	Table 1: <[DPK2003] QSO JHHMM+DDMM abs N.NNN> N=18. Tables 2-14: <[DPK2003] QSO JHHMM+DDMM abs N.NNNNNN> N=121.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPL2003]
[DPL2003]	(Dahle+Pedersen+Lilje+, 2003)= (WL)
Write:	<<[DPL2003] WL JHHMM.m+DDMM>> <<[DPL2003] JHHMMSS.s+DDMMSS>>
N:	3+2
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=3 Weak Lensing (WL in the format) detected concentrations in the fields of 3 ACO: ACO 959, ACO 1705, ACO 1722. A giant elliptical galaxy is found in the field of ACO 1705 'J131231.1+725054', and near this galaxy a gravitationally lensed arc 'J131232.6+725055'.
Ref:	=2003ApJ...591..662D
by	DAHLE H. , PEDERSEN K., LILJE P.B., MADDOX S.J., KAISER N.
	Astrophys. J., 591, 662-676 (2003)
	Weak gravitational lensing by a sample of X-ray-luminous clusters of galaxies. III. Serendipitous weak lensing detections of dark and luminous mass concentrations.
o	Paragr. 3.1: Sources A to D in ACO 959 not identified in SIMBAD.
o	Table 1: <[DPL2003] WL JHHMM.m+DDMM> N=3. Text: <[DPL2003] JHHMMSS.s+DDMMSS> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPM2001]
[DPM2001]	(D'Amico+Possenti+Manchester+, 2001)
Write:	<<[DPM2001] J1701-30A>>
N:	6
Object:	ms Psr (SIMBAD class: Pulsar)
Stat:	is completely incorporated in Simbad
Note:	N=6 millisecond pulsars in NGC 6266, also found as PSR J1701-3006A to F. The 3 first millisecond pulsars A to C have been discovered by D'Amico+ in 2001, astro-ph/0105122, not published.
in source:	NGC 6366 = M 62
Ref:	=2002IAUC.7783....1J
by	JACOBY B.A. , CHANDLER A.M., BACKER D.C., ANDERSON S.B., KULKARNI S.R.
	IAU Circ., 7783, 1-None (2002)
	Pulsars in M62.
o	The 3 first millisecond pulsars A to C have been discovered by D'Amico+ in 2001, Astro-ph/0105122, not published.
o	<[DPM2001] J1701-30A> (Nos D-F) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPM2007]
[DPM2007]	(De Marchi+Poretti+Montaldo+, 2007)
Write:	<<[DPM2007] NNNNN-NN>>
N:	260
Object:	V* in Cluster of * (SIMBAD class: Variable* = Variable Star)
Note:	CFHT, San Pedro Martir 2.1m telescope, and Loiano 1.5m telescope observations. Discovery of 260 new variable stars in NGC 6791.
in source:	NGC 6791
Ref:	=2007A&A...471..515D
by	DE MARCHI F. , PORETTI E., MONTALTO M., PIOTTO G., DESIDERA S., BEDIN L.R., CLAUDI R., ARELLANO FERRO A., BRUNTT H., STETSON P.B.
	Astron. Astrophys., 471, 515-526 (2007)
	Variable stars in the open cluster NGC 6791 and its surrounding field.
o	Paragraph 4.3 NGC 6971 is a probable misprint for NGC 6791. Paragraph 4.1 00122_4 is a probable misprint for 01122_4. Paragraph 4.6 001606_1 is a probable misprint for 01606_11.
o	Catalog: <[DPM2007] NNNNN-NN> N=260.
=E=	Catalogue in electronic form as J/A+A/471/515
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPM2010]
[DPM2010]	(De Marchi+Poretti+Montalto+, 2010)
Write:	<<[DPM2010] NNNNN-N>>
N:	595
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	ESO-MPI 2.2m telescope WFI observations of N=595 variable stars in the open cluster NGC 6253.
in source:	NGC 6253
Ref:	=2010A&A...509A..17D
by	DE MARCHI F. , PORETTI E., MONTALTO M., DESIDERA S., PIOTTO G.
	Astron. Astrophys., 509A, 17-17 (2010)
	The first search for variable stars in the open cluster NGC 6253 and its surrounding field.
o	Tables A.1-A10: <[DPM2010] NNNNN-N> N=595.
Ref:	=2011A&A...535A..39M
by	MONTALTO M. , VILLANOVA S., KOPPENHOEFER J., PIOTTO G., DESIDERA S., DE MARCHI F., PORETTI E., BEDIN L.R., SAVIANE I.
	Astron. Astrophys., 535A, 39-39 (2011)
	VLT multi-epoch radial velocity survey toward NGC 6253. Analysis of three transiting planetary candidates.
o	Tables 9-10: <[DPM2010] NNNNN-N> N=139.
=E=	Catalogue in electronic form as J/A+A/509/A17
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPM2014]
[DPM2014]	(Duc+Paudel+Mcdermid+, 2014)
Write:	<<[DPM2014] NGCNNNN-WW>> <<[DPM2014] NGC5557-WN>>
N:	4+3
Object:	Tidal dwarf galaxy candidate (SIMBAD class: Galaxy)
Note:	Gemini-North GMOS spectroscopy of N=7 satellite galaxies in the vicinity of five early-type galaxies.
in source:	NGC 2764
in source:	NGC 3193
in source:	NGC 5485
in source:	NGC 5557
Ref:	=2014MNRAS.440.1458D
by	DUC P.-A. , PAUDEL S., McDERMID R.M., CUILLANDRE J.-C., SERRA P., BOURNAUD F., CAPPELLARI M., EMSELLEM E.
	Mon. Not. R. Astron. Soc., 440, 1458-1469 (2014)
	Identification of old tidal dwarfs near early-type galaxies from deep imaging and HI observations.
o	Fig. 1, Table 1: <[DPM2014] NGCNNNN-WW> N=4, <[DPM2014] NGC5557-WN> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPN2008]
[DPN2008]	(Day-Jones+Pinfield+Napiwotzki+, 2008)
Write:	<<[DPN2008] UCDc-N>> <<[DPN2008] WDc-N>>
N:	8+8
Object:	* + * in Pair (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Use of 2MASS and SuperCOSMOS archives in the Southern hemisphere.
Ref:	=2008MNRAS.388..838D
by	DAY-JONES A.C. , PINFIELD D.J., NAPIWOTZKI R., BURNINGHAM B., JENKINS J.S., JONES H.R.A., FOLKES S.L., WEIGHTS D.J., CLARKE J.R.A.
	Mon. Not. R. Astron. Soc., 388, 838-848 (2008)
	Discovery of a widely separated ultracool dwarf-white dwarf binary.
o	Table 2: <[DPN2008] UCDc-N> (Nos 1 to 8), <[DPN2008] WDc-N> (Nos 1 to 8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DPOSS
DPOSS	(Digital Palomar Sky Survey)
*****	Avoid the usage of DPOSS, prefer PSS
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [DPP2015]
[DPP2015]	(Donovan Meyer+Peek+Putman+, 2015)
Write:	<<[DPP2015] NN>>
N:	98
Object:	HI Cloud (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	Selection of N=98 compact HI clouds with UV counterparts to identify dwarf galaxy candidates. Use of archival GALEX data. Use of GALFA-HI and ALFALFA blind HI surveys.
Ref:	=2015ApJ...808..136D
by	DONOVAN MEYER J. , PEEK J.E.G., PUTMAN M., GRCEVICH J.
	Astrophys. J., 808, 136 (2015)
	Finding gas-rich dwarf galaxies betrayed by their ultraviolet emission.
o	Table 1: <[DPP2015] NN> (Nos 1-98).
=E=	Catalogue in electronic form as J/ApJ/808/136
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPP2017]
[DPP2017]	(Damiani+Pillitteri+Prisinzano, 2017)
Write:	<<[DPP2017] NNN>>
N:	994
Object:	(X) + Poss. YSO (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	XMM-Newton EPIC and Chandra ACIS-I observations of N=994 sources in the North America and Pelican complex.
in source:	IC 5070 = NAME Pelican Nebula
in source:	NGC 7000 = NAME North America Nebula
Ref:	=2017A&A...602A.115D
by	DAMIANI F. , PILLITTERI I., PRISINZANO L.
	Astron. Astrophys., 602A, 115-115 (2017)
	X-ray survey of the North-America and Pelican star-forming complex (NGC 7000/IC 5070).
o	Tables 3-4: <[DPP2017] NNN> (Nos 1-721). Table 5: <[DPP2017] NNN> (Nos 722-994).
=E=	Catalogue in electronic form as <J/A+A/602/A115/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPP99]
[DPP99]	(Drinkwater+Proust+Parker+, 1999)
Write:	<<[DPP99] HHMMSS.s+DDMMSS>>
N:	306
Object:	G in Supercluster (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Some corections of coordinates and redshifts are found in 2004PASA...21...89D.
in source:	NAME SHAPLEY SUPERCL
Ref:	=1999PASA...16..113D
by	DRINKWATER M.J. , PROUST D., PARKER Q.A., QUINTANA H., SLEZAK E.
	Publications - Astron. Soc. Australia, 16, 113-123 (1999)
	New structure in the Shapley supercluster.
o	see also corrections given in table 2 of 2004PASA.21.89D.
o	Table 2: <[DPP99] HHMMSS.s+DDMMSS> N=306.
=E=	Catalogue in electronic form as J/other/PASA/16.113
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPR2015]
[DPR2015]	(Draskovic+Parker+Reid+, 2015)
Write:	<<[DPR2015] N>>
N:	4
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	SAAO 1.9 m telescope spectroscopy of N=4 planetary nebulae (PNe) in the field of the Small Magellanic Cloud (SMC).
in source:	NAME SMC
Ref:	=2015MNRAS.452.1402D
by	DRASKOVIC D. , PARKER Q.A., REID W.A., STUPAR M.
	Mon. Not. R. Astron. Soc., 452, 1402-1411 (2015)
	Four new planetary nebulae towards the Small Magellanic Cloud.
o	Table 3: <[DPR2015] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPR2019]
[DPR2019]	(Dewangan+Pirogov+Ryabukhina+, 2019)
Write:	<<[DPR2019] N>>
N:	5
Object:	Dense Core (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	OSO 20-m telescope 13CO(1-0), 18CO(1-0), and CS(2-1) line observations of Sh 2-242. N=5 dense cores detected in the CS and 18CO maps.
in source:	SH 2-242
Ref:	=2019ApJ...877....1D
by	DEWANGAN L.K. , PIROGOV L.E., RYABUKHINA O.L., OJHA D.K., ZINCHENKO I.
	Astrophys. J., 877, 1-1 (2019)
	Observational signatures of end-dominated collapse in the S242 filamentary structure.
o	The clumps PGCC G181.84+00.31aN are not in SIMBAD.
o	Fig. 6(c), Table 2: <[DPR2019] N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPS2018]
[DPS2018]	(Dar+Parihar+Saleh+, 2018) (Not yet in Simbad)
Write:	<<[DPS2018] IDNNN>>
N:	60
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Vainu Bappu 1.3m JCB telescope observations of N=60 variable stars in M37.
in source:	NGC 2099 = M37
Ref:	=2018RAA....18..155D
by	DAR A.A. , PARIHAR P.S., SALEH P., MALIK M.A.
	RAA, 18, 155-155 (2018)
	Variable stars in M37.
o	Fig. 3, Table 2: <[DPS2018] IDNNN> N=60 among (Nos ID002-ID303).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPS86]
[DPS86]	(Downes+Pauls+Salter, 1986)
Write:	<<[DPS86] BHHMM+DDd>>
N:	7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Effelsberg 100m telescope 5GHz observations of the field of W 50.
Ref:	=1986MNRAS.218..393D
by	DOWNES A.J.B. , PAULS T., SALTER C.J.
	Mon. Not. R. Astron. Soc., 218, 393-407 (1986)
	The supernova remnant W 50 at 5 GHz.
o	Table 1: <[DPS86] BHHMM+DDd> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPS88]
[DPS88]	(Da Costa+Pellegrini+Sargent+, 1988)= (dC88)
Write:	<<[DPS88] N>>
N:	4
Object:	Void (SIMBAD class: Void = Underdense Region of the Universe)
Stat:	is completely incorporated in Simbad
Note:	N=4 Voids in the SSRS survey. See also [EP97b] voids in the SSRS2 survey
Ref:	=1988ApJ...327..544D
by	DA COSTA L.N. , PELLEGRINI P.S., SARGENT W.L.W., TONRY J., DAVIS M., MEIKSIN A., LATHAM D.W., MENZIES J.W., COULSON I.A.
	Astrophys. J., 327, 544-560 (1988)
	The Southern Sky Redshift Survey.
o	Table 1: <[DPS88] N> N=4
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DPT00
DPT00	(De Buizer+Pina+Telesco, 2000)
Write:	<<DPT00 GLLL.ll+B.bb N>> <<DPT00 GLLL.lll+B.bbb NA>>
N:	33+3
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	N=33 multiple Mid-infrared sources 'N' in the same 'GLLL.ll+B.bb' or 'GLLL.lll+B.bbb' site. G339.88-1.26 1 is divided in 3 IR peaks (Nos 1A to 1C). See also [DRT2003] and DRT05.
Ref:	=2000ApJS..130..437D
by	DE BUIZER J.M. , PINA R.K., TELESCO C.M.
	Astrophys. J., Suppl. Ser., 130, 437-461 (2000)
	Mid-infrared imaging of star-forming regions containing methanol masers.
o	Table 2, Figs: <DPT00 GLLL.ll+B.bb N>, <DPT00 GLLL.lll+B.bbb N>, N=33.
Ref:	=2002ApJ...564..327D
by	DE BUIZER J.M. , WALSH A.J., PINA R.K., PHILLIPS C.J., TELESCO C.M.
	Astrophys. J., 564, 327-332 (2002)
	High-resolution mid-infrared imaging of G339.88-1.26.
o	Table 1, Fig.1: <DPT00 G339.88-1.26 1A> (Nos 1A to 1C).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DPT2019]
[DPT2019]	(DeFelippis+Putman+Tollerud, 2019)
Write:	<<[DPT2019] GLLL.ll+BB.bb+VVV>> <<[DPT2019] LLL.ll+BB.bb+VVV>> (not recognised by Simbad, but found in literature)
N:	690
Object:	(HI) + Poss. Dwarf G (SIMBAD class: HI = HI (21cm) Source)
Note:	N=690 dwarf galaxy candidates from the Galactic Arecibo L-Band Feed Array Survey (GALFA) DR2. See also [SPG2012].
Ref:	=2019ApJ...879...22D
by	DEFELIPPIS D. , PUTMAN M., TOLLERUD E.
	Astrophys. J., 879, 22-22 (2019)
	A correlated search for local dwarf galaxies in GALFA-H I and Pan-STARRS.
o	Table 2: <[DPT2019] GLLL.ll+BB.bb+VVV> N=690.
=E=	Catalogue in electronic form as <J/ApJ/879/22/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DPV
DPV	(Duerbeck+Pollacco+Verbunt+)
Write:	<<DPV N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Sakurai's object is surrounded by a faint planetary nebula.
Ref:	=1996IAUC.6328Q...1D
by	DUERBECK H.W. , POLLACCO D., VERBUNT F., GEERTSEMA G.
	IAU Circ., 6328, 1-None (1996)
	Novalike variable in Sagittarius.
o	<DPV N> (No. 1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DPW87]
[DPW87]	(Donnelly+Partridge+Windhorst, 1987)
Write:	<<[DPW87] NN/WN>>
N:	58
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=58 sources 'NN', in 3 fields 'W1, W2, W3'. In the format the letter 'W' stands for the Wind field name
in source:	NAME Lynx Region
Ref:	=1987ApJ...321...94D
by	DONNELLY R.H. , PARTRIDGE R.B., WINDHORST R.A.
	Astrophys. J., 321, 94-112 (1987)
	6 centimeter radio source counts and spectral index studies down to 0.1 millijansky.
o	Table 2: <[DPW87] NN/W1> N=32, <[DPW87] NN/W2> N=11, <[DPW87] NN/W3> N=15.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DQ90]
[DQ90]	(De Souza+Quintana, 1990)
Write:	<<[DQ90] NN>> <<[DQ90] BNN>>
N:	24+19
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ESO 3.6m telescope OPTOPUS observation. Search of members of the Group 'NAME NGC 4782-NGC 4783 Group'. Source names 'BNN' are background objects.
in source:	NAME NGC 4782-NGC 4783 GROUP
Ref:	=1990AJ.....99.1065D
by	DE SOUZA R. , QUINTANA H.
	Astron. J., 99, 1065-1070 (1990)
	The NGC 4782/3 dumbbell massive group.
o	Table I(a, b): <[DQ90] NN> (Nos 1-13, 14-24). Table I(c): <[DQ90] BNN> (Nos B1-B19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DR
DR	(Downes+Rinehart)
Write:	<<DR NN>> <<DR 21(OH)>>
N:	21
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	(Nos 1-27), Nos 2, 8, 14, 24, 25, 26 are not defined.
Ref:	=1966ApJ...144..937D
by	DOWNES D. , RINEHART R.
	Astrophys. J., 144, 937-942 (1966)
	Microwave observations of the Cyg X region.
o	Table 1: <DR NN> N=21 among (Nos 1-27)
Details on Acronym: DR
DR	(D'odorico+Rosa)
Write:	<<NAME DR N>>
N:	1
Object:	WR (SIMBAD class: WolfRayet* = Wolf-Rayet)
in source:	IC 1613
Ref:	=1982A&A...105..410D
by	D'ODORICO S. , ROSA M.
	Astron. Astrophys., 105, 410-412 (1982)
	Wolf-Rayet stars in extragalactic HII regions: discovery of a peculiar WR in IC 1613/#3.
o	<NAME DR 1>
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [DR2006]
[DR2006]	(Delain+Rudnick) (Not yet in Simbad)
Write:	<<[DR2006] JHHMM+DD>> <<[DR2006] HHMM+DD>> (not recognised by Simbad, but found in literature)
N:	3
Object:	(Radio) (SIMBAD class: Radio = Radio Source)
Note:	Discovery of diffuse radio sources in the Westerbork Northern Sky Survey (WENSS).
Ref:	=2006AN....327..561D
by	DELAIN K.M. , RUDNICK L.
	Astron. Nachr., 327, 561-562 (2006)
	Diffuse radio sources in groups and poor clusters.
o	Fig.2: <[DR2006] JHHMM+DD> N=3.
Details on Acronym: dr5EGal
dr5EGal	(SDSS DR5, Equatorial, Galaxy)
Write:	<<dr5EGal NNNNN NNNNNN>>
N:	129985
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Note:	Search for groups of galaxies in the Equatorial and Northern part of the SDSS DR5 survey (dr5EGr and dr5NGr catalogues). N=129985 galaxies in the Equatorial groups.
Ref:	=2008A&A...479..927T
by	TAGO E. , EINASTO J., SAAR E., TEMPEL E., EINASTO M., VENNIK J., MUELLER V.
	Astron. Astrophys., 479, 927-937 (2008)
	Groups of galaxies in the SDSS Data Release 5. A group-finder and a catalogue.
o	Table 3a: <dr5EGr NNNNN> (Nos 1-17143). Table 3b: <dr5NGr NNNNN> (Nos 1-33219). Table 3c: <dr5EGal NNNNN NNN> N=129985. Table 3d: <dr5NGal NNNNN NNN> N=257078.
=E=	Catalogue in electronic form as J/A+A/479/927
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: dr5EGr
dr5EGr	(SDSS DR5, Equatorial, Group)
Write:	<<dr5EGr NNNNN>>
N:	17143
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	Search for groups of galaxies in the Equatorial and Northern part of the SDSS DR5 survey (dr5EGr and dr5NGr catalogues). See also dr5EGal catalogue of galaxies in Equatorial groups.
Ref:	=2008A&A...479..927T
by	TAGO E. , EINASTO J., SAAR E., TEMPEL E., EINASTO M., VENNIK J., MUELLER V.
	Astron. Astrophys., 479, 927-937 (2008)
	Groups of galaxies in the SDSS Data Release 5. A group-finder and a catalogue.
o	Table 3a: <dr5EGr NNNNN> (Nos 1-17143). Table 3b: <dr5NGr NNNNN> (Nos 1-33219). Table 3c: <dr5EGal NNNNN NNN> N=129985. Table 3d: <dr5NGal NNNNN NNN> N=257078.
=E=	Catalogue in electronic form as J/A+A/479/927
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: dr5NGal
dr5NGal	(SDSS DR5, North, Galaxy)
Write:	<<dr5NGal NNNNN NNNNNN>>
N:	257078
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Note:	Search for groups of galaxies in the Equatorial and Northern part of the SDSS DR5 survey (dr5EGr and dr5NGr catalogues). N=257078 galaxies in the Northern groups.
Ref:	=2008A&A...479..927T
by	TAGO E. , EINASTO J., SAAR E., TEMPEL E., EINASTO M., VENNIK J., MUELLER V.
	Astron. Astrophys., 479, 927-937 (2008)
	Groups of galaxies in the SDSS Data Release 5. A group-finder and a catalogue.
o	Table 3a: <dr5EGr NNNNN> (Nos 1-17143). Table 3b: <dr5NGr NNNNN> (Nos 1-33219). Table 3c: <dr5EGal NNNNN NNN> N=129985. Table 3d: <dr5NGal NNNNN NNN> N=257078.
=E=	Catalogue in electronic form as J/A+A/479/927
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: dr5NGr
dr5NGr	(SDSS DR5, North, Group)
Write:	<<dr5NGr NNNNN>>
N:	33219
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	Search for groups of galaxies in the Equatorial and Northern part of the SDSS DR5 survey (dr5EGr and dr5NGr catalogues). See also dr5NGal catalogue of galaxies in Northern groups.
Ref:	=2008A&A...479..927T
by	TAGO E. , EINASTO J., SAAR E., TEMPEL E., EINASTO M., VENNIK J., MUELLER V.
	Astron. Astrophys., 479, 927-937 (2008)
	Groups of galaxies in the SDSS Data Release 5. A group-finder and a catalogue.
o	Table 3a: <dr5EGr NNNNN> (Nos 1-17143). Table 3b: <dr5NGr NNNNN> (Nos 1-33219). Table 3c: <dr5EGal NNNNN NNN> N=129985. Table 3d: <dr5NGal NNNNN NNN> N=257078.
=E=	Catalogue in electronic form as J/A+A/479/927
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Dra
Dra	(Draco)
*****	Avoid the usage of Dra, prefer [ALS82]
Origin	of the Acronym: L (1993ApJ...410..260S)
Details on Acronym: [DRA2010]
[DRA2010]	(Donley+Rieke+Alexander+, 2010)= (IRBG)
Write:	<<[DRA2010] IRBGNN>>
N:	13
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRS observations of N=13 IR-bright/optically-faint galaxies (IRBGs).
Ref:	=2010ApJ...719.1393D
by	DONLEY J.L. , RIEKE G.H., ALEXANDER D.M., EGAMI E., PEREZ-GONZALEZ P.G.
	Astrophys. J., 719, 1393-1407 (2010)
	The AGN, star-forming, and morphological properties of luminous IR-bright/optically-faint galaxies.
o	Tables 1-4: <[DRA2010] IRBGNN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRA2013]
[DRA2013]	(Dzib+Rodriguez+Araudo+, 2013)
Write:	<<[DRA2013] B59 VLA N>>
N:	6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Archival VLA continuum observations at 8.3 GHz of N=6 compact sources toward the dense core Barnard 59, in the Pipe Nebula.
in source:	Barnard 59
Ref:	=2013RMxAA..49..345D
by	DZIB S.A. , RODRIGUEZ L.F., ARAUDO A.T., LOINARD L.
	RMxAA, 49, 345 (2013)
	Radio sources embedded in the dense core B59, the "mouthpiece" of the Pipe Nebula.
o	Fig. 1, Table 1: <[DRA2013] B59 VLA N> (Nos 1-6).
Details on Acronym: Draco
Draco	(Draco)
*****	Avoid the usage of Draco, prefer [ALS82]
Origin	of the Acronym: L (2008MNRAS.384.1178B)
Details on Acronym: Draco
Draco	(Draco)
*****	Avoid the usage of Draco, prefer [BS61]
Origin	of the Acronym: L (2008MNRAS.384.1178B)
Details on Acronym: DRaGONS
DRaGONS	(Distant Radio Galaxies Optically Non-detected in the SDSS)
Write:	<<DRaGONS JHHMM+DDMMa>>
N:	117+34
Object:	rG (SIMBAD class: RadioG = Radio Galaxy)
Note:	DRaGONS Survey: N=117 bright FIRST radio sources without a SDSS counterpart. N=22 sources have a double or triple lobe morphology (letter 'a' at the end of the format). N=34 sources are nondetections.
Ref:	=2006ApJ...649...63S
by	SCHMIDT S.J. , CONNOLLY A.J., HOPKINS A.M.
	Astrophys. J., 649, 63-78 (2006)
	The DRaGONS survey: a search for high-redshift radio galaxies and heavily obscured active galactic nuclei.
o	Tables 1, 2: <DRaGONS JHHMM+DDMMa> N=117+34.
=E=	Catalogue in electronic form as J/ApJ/649/63
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DRAO
DRAO	(Dominion Radio Astrophysical Observatory) (Not yet in Simbad)
*****	Avoid the usage of DRAO, prefer [BGT2011]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DRAO
DRAO	(Dominion Radio Astrophysical Observatory) (Not yet in Simbad)
*****	Avoid the usage of DRAO, prefer [GTS2010]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DRB2005]
[DRB2005]	(De Becker+Rauw+Blomme+, 2005)
Write:	<<[DRB2005] NN>>
N:	31
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of the field around HD 167971.
Ref:	=2005A&A...437.1029D
by	DE BECKER M. , RAUW G., BLOMME R., PITTARD J.M., STEVENS I.R., RUNACRES M.C.
	Astron. Astrophys., 437, 1029-1046 (2005)
	An XMM-Newton observation of the multiple system HD 167971 (O5-8V + O5-8V + (O8I)) and the young open cluster NGC 6604.
o	Table 6: <[DRB2005] NN> (Nos 1-31).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRB2015]
[DRB2015]	(Downes+Roman-Zuniga+Ballesteros-Paredes+, 2015)
Write:	<<[DRB2015] NN>>
N:	21
Object:	Poss. Brown Dwarf (SIMBAD class: BrownD*_Candidate = Brown Dwarf Candidate)
Stat:	is completely incorporated in Simbad
Note:	GTC OSIRIS spectroscopy of N=21 brown dwarf candidates in Orion OB1a and 25 Orionis group.
in source:	NAME 25 ORI GROUP
in source:	NAME Ass ORI OB 1a
Ref:	=2015MNRAS.450.3490D
by	DOWNES J.J. , ROMAN-ZUNIGA C., BALLESTEROS-PAREDES J., MATEU C., BRICENO C., HERNANDEZ J., PETR-GOTZENS M.G., CALVET N., HARTMANN L., MAUCO K.
	Mon. Not. R. Astron. Soc., 450, 3490-3502 (2015)
	The number fraction of discs around brown dwarfs in Orion OB1a and the 25 Orionis group.
o	[DRB2015] 1, 7, 11, 13, 16, 20 not created in Simbad (no coordinates provided in the article)
o	Table 1: <[DRB2015] NN> (Nos 1-21).
=E=	Catalogue in electronic form as <J/MNRAS/450/3490/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRB2020]
[DRB2020]	(Dabhade+Rottgering+Bagchi+, 2020)
Write:	<<[DRB2020] NNN>>
N:	239
Object:	Giant Radio G (SIMBAD class: RadioG = Radio Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=239 giant radio galaxies (GRGs), in the LOFAR Two-metre Sky Survey first data release images.
Ref:	=2020A&A...635A...5D
by	DABHADE P. , ROTTGERING H.J.A., BAGCHI J., SHIMWELL T.W., HARDCASTLE M.J., SANKHYAYAN S., MORGANTI R., JAMROZY M., SHULEVSKI A., DUNCAN K.J.
	Astron. Astrophys., 635A, 5-5 (2020)
	Giant radio galaxies in the LOFAR Two-metre Sky Survey. I. Radio and environmental properties.
o	Figs A.1-A.8, Table A.1: <[DRB2020] NNN> (Nos 1-239).
=E=	Catalogue in electronic form as <J/A+A/635/A5/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRB94]
[DRB94]	(Della Valle+Rosino+Bianchini+, 1994)
Write:	<<[DRB94] NN>>
N:	10
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Stat:	is completely incorporated in Simbad
in source:	M 33 = NGC 598
Ref:	=1994A&A...287..403D
by	DELLA VALLE M. , ROSINO L., BIANCHINI A., LIVIO M.
	Astron. Astrophys., 287, 403-409 (1994)
	The nova rate in galaxies of different Hubble types.
o	Table 1: <[DRB94] NN> (Nos 1-10)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRC2011]
[DRC2011]	(Diaz+Ryan-Weber+Cooke+, 2011)
Write:	<<[DRC2011] JHHMMSS.ss+DDMMSS.ss>>
N:	3
Object:	LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 spectroscopy of N=3 LAEs near QSO J1030+0524. Use of HST ACS images.
Ref:	=2011MNRAS.418..820D
by	DIAZ C.G. , RYAN-WEBER E.V., COOKE J., PETTINI M., MADAU P.
	Mon. Not. R. Astron. Soc., 418, 820-827 (2011)
	A galaxy as the source of a C IV absorption system close to the epoch of reionization.
o	Figs 1-3, Table 1: <[DRC2011] JHHMMSS.ss+DDMMSS.ss> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DRCG
DRCG	(Dressler, Cluster of G)= (DC)
Write:	<<DRCG HHMM+DD>>
N:	17
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Ref:	=1980ApJS...42..565D
by	DRESSLER A.
	Astrophys. J., Suppl. Ser., 42, 565-609 (1980)
	A catalog of morphological types in 55 rich clusters of galaxies.
o	Table 1: <DRCG HHMM-DD> N=17. Table 2: <[D80] ACO NNNN NNN>, <[D80] DRCG HHMM-DD NNN>, <[D80] CEN NN>, G in 56 ClG, N about 6000.
=E=	Catalogue in electronic form as VII/174
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [DRD2009]
[DRD2009]	(Decarli+Reynolds+Dotti, 2009)
Write:	<<[DRD2009] NN>>
N:	54
Object:	(IR) + G (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	K-band photometry of N=54 sources of the field of SDSS J092712.65+294344.0. Use of GALEX and SDSS archival data.
in source:	SDSS J092712.65+294344.0
Ref:	=2009MNRAS.397..458D
by	DECARLI R. , REYNOLDS M.T., DOTTI M.
	Mon. Not. R. Astron. Soc., 397, 458-466 (2009)
	A photometric study of the field around the candidate recoiling/binary black hole SDSS J092712.65+294344.0.
o	Table 2: <[DRD2009] NN> N=54 among (Nos 1-77).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRE2010]
[DRE2010]	(Dunham+Rosolowsky+Evans+, 2010)
Write:	<<[DRE2010] NN>>
N:	55
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=55 mm continuum sources in the Gemini OB1 molecular cloud. Use of data from the Bolocam Galactic Plane Survey. See also BGPS.
in source:	NAME ASS GEM OB 1-
Ref:	=2010ApJ...717.1157D
by	DUNHAM M.K. , ROSOLOWSKY E., EVANS N.J., CYGANOWSKI C.J., AGUIRRE J., BALLY J., BATTERSBY C., BRADLEY E.T., DOWELL D., DROSBACK M., GINSBURG A., GLENN J., HARVEY P., MERELLO M., SCHLINGMAN W., SHIRLEY Y.L., STRINGFELLOW G.S., WALAWENDER J., WILLIAMS J.P.
	Astrophys. J., 717, 1157-1180 (2010)
	The Bolocam Galactic Plane Survey. III. Characterizing physical properties of massive star-forming regions in the Gemini OB1 molecular cloud.
o	Table 3: <[DRE2010] NN> (Nos 1-55).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRF2003]
[DRF2003]	(De Laney+Rudnick+Fesen+, 2004) (Not yet in Simbad)
Write:	<<[DRF2003] NNN>>
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Chandra observations are used to search for knots and filaments with a proper motion in Cas A.
in source:	NAME Cas A
Ref:	=2004ApJ...613..343D
by	DELANEY T. , RUDNICK L., FESEN R.A., JONES T.W., PETRE R., MORSE J.A.
	Astrophys. J., 613, 343-348 (2004)
	Kinematics of X-Ray-emitting components in Cassiopeia A.
o	Table 1: <[DRF2003] NNN> (Nos 1-261).
=E=	Catalogue in electronic form as J/ApJ/613/343
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DRG
DRG	(Distant Red Galaxy) (Not yet in Simbad)
*****	Avoid the usage of DRG, prefer [PSL2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DRG
DRG	(Distant Red Galaxy)
*****	Avoid the usage of DRG, prefer [LSE2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DRG2004]
[DRG2004]	(Dirsch+Richtler+Geisler+, 2004)
Write:	<<[DRG2004] NN:NNN>>
N:	418+73
Object:	GlCl + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Search for globular clusters around NGC 1399 with FORS2 and the Mask Exchange Unit (MXU) at the ESO VLT. In the format the first number stands for the mask, the second for the aperture number on the maks assigned during the extraction process.
in source:	NGC 1399
Ref:	=2004AJ....127.2114D
by	DIRSCH B. , RICHTLER T., GEISLER D., GEBHARDT K., HILKER M., ALONSO M.V., FORTE J.C., GREBEL E.K., INFANTE L., LARSEN S., MINNITI D., REJKUBA M.
	Astron. J., 127, 2114-2132 (2004)
	The globular cluster system of NGC 1399. III. VLT spectroscopy and database.
o	Tables 3, 4: <[DRG2004] NN:NNN> N=468+73.
=E=	Catalogue in electronic form as J/AJ/127/2114
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRG92]
[DRG92]	(Downes+Radford+Guilloteau+, 1992)= (GMC)
Write:	<<[DRG92] AN>> <<[DRG92] A'>>
N:	6+7
Object:	Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=6 HCN Clouds in IC 342: (Nos A-E, D'). Clouds B, C, E, are divided in several smaller clouds AN. The positions of the clouds show no significant differences in CO maps (ref. 2000ApJ...531..200M).
in source:	IC 342
Ref:	=1992A&A...262..424D
by	DOWNES D. , RADFORD S.J.E., GUILLOTEAU S., GUELIN M., GREVE A., MORRIS D.
	Astron. Astrophys., 262, 424-432 (1992)
	HCN in the center of the galaxy IC 342.
o	Fig.1, Table 1: <[DRG92] A> (Nos A-E).
Ref:	=2001ApJ...551..687M
by	MEIER D.S. , TURNER J.L.
	Astrophys. J., 551, 687-701 (2001)
	Molecular gas and star formation in the nucleus of IC 342: C^{18}O and millimeter continuum imaging.
o	Table 4: <[DRG92] AN> (Nos B1-B2, C1-C3, E1-E2) added.
Ref:	=2005ApJ...618..259M
by	MEIER D.S. , TURNER J.L.
	Astrophys. J., 618, 259-280 (2005)
	Spatially resolved chemistry in nearby galaxies. I. The center of IC 342.
o	Table 3: <[DRG92] A'> (No. D') added. Fig.3: <[MT2005] Cloud A> (No. N).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRH2012]
[DRH2012]	(Da Rio+Robberto+Hillenbrand+, 2012)
Write:	<<[DRH2012] NNNN>>
N:	1743
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	ESO/MPG 2.2m telescope WFI observations of N=1743 stars in the Orion Nebula Cluster. See also [DRS2009].
in source:	NAME ONC
Ref:	=2012ApJ...748...14D
by	DA RIO N. , ROBBERTO M., HILLENBRAND L.A., HENNING T., STASSUN K.G.
	Astrophys. J., 748, 14 (2012)
	The initial mass function of the Orion Nebula Cluster across the H-burning limit.
o	Table 3: <[DRH2012] NNNN> (Nos 1-1743).
=E=	Catalogue in electronic form as J/ApJ/748/14
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Dril
Dril	(Drilling)
Write:	<<Dril NN>>
N:	51
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1977AJ.....82..714D
by	DRILLING J.S.
	Astron. J., 82, 714-717 (1977)
	UBV photometry of stars in a region near the South Galactic Pole.
o	Table II: <Dril NN> (Nos 1-51)
Details on Acronym: [DRJ2018]
[DRJ2018]	(Desprez+Richard+Jauzac+, 2018) (Not yet in Simbad)
Write:	<<[DRJ2018] ANNN-GGLN>> <<[DRJ2018] MACSNNNN-GGLN>> <<[DRJ2018] MS2137-GGL1>> <<[DRJ2018] RX JNNNN-GGLN>> <<[DRJ2018] SMACS2248-GGLN>> <<[DRJ2018] RX J2129 A.N>> <<[DRJ2018] RX J2129 N.N>> <<[DRJ2018] MACS0329 A.N>> <<[DRJ2018] MACS0329 N.N>> <<[DRJ2018] MACS1149 A.N>> <<[DRJ2018] MACS1149 NN.N>>
N:	24+12+18+69
Object:	LeG + LI? (SIMBAD class: GravLensSystem_Candidate = Gravitational Lens System (lens+images) Candidate)
Note:	Catalogue of N=24 candidate galaxy-galaxy lensing (GGL) identified from HST images in the outskirts of the massive galaxy clusters from the CLASH survey. Detailed study (strong-lensing mass reconstructions) for three of them, detected in the RX J2129, MACS J0329, and MACS J1149 clusters. Use of archival VLT VIMOS data.
Ref:	=2018MNRAS.479.2630D
by	DESPREZ G. , RICHARD J., JAUZAC M., MARTINEZ J., SIANA B., CLEMENT B.
	Mon. Not. R. Astron. Soc., 479, 2630-2648 (2018)
	Galaxy-galaxy lensing in the outskirts of CLASH clusters: constraints on local shear and testing mass-luminosity scaling relation.
o	Table A1: <[DRJ2018] A209-GGLN> (Nos 1-2), <[DRJ2018] A383-GGL1> N=1, <[DRJ2018] MACS0429-GGLN> (Nos 1-2), <[DRJ2018] MACS0329-GGL1> N=1, <[DRJ2018] MACS0416-GGLN> (Nos 1-3), <[DRJ2018] MACS0717-GGL1> N=1, <[DRJ2018] MACS0744-GGL1> N=1, <[DRJ2018] MACS1115-GGL1> N=1, <[DRJ2018] MACS1149-GGLN> (Nos 1-4), <[DRJ2018] MS2137-GGL1> N=1, <[DRJ2018] RX J1347-GGLN> N=3, <[DRJ2018] RX J2129-GGL1> N=1, <[DRJ2018] SMACS2248-GGLN> (Nos 1-3). Table B1: <[DRJ2018] RX J2129 A.N> (Nos A.1-A.4), <[DRJ2018] RX J2129 N.N> (Nos 1.1-5.2). Table B3: <[DRJ2018] MACS0329 A.N> (Nos A.1-B.4), <[DRJ2018] MACS0329 N.N> (Nos 1.1-3.3). Table B5: <[DRJ2018] MACS1149 A.N> (Nos A.1-A.4), <[DRJ2018] MACS1149 NN.N> (Nos 1.1-34.3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRK2018]
[DRK2018]	(Dzib+Rodriguez+Karuppusamy+, 2018)= (VLA)
Write:	<<[DRK2018] VLA JHHMMSS.ss+DDMMSS.s>>
N:	27
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 4-8GHz and 8-12GHz observations of N=27 radio sources towards PSR J1813-1749 and HESS J1813-178. Use of NRAO VLA archival data at 5.5GHz.
Ref:	=2018ApJ...866..100D
by	DZIB S.A. , RODRIGUEZ L.F., KARUPPUSAMY R., LOINARD L., MEDINA S.-N.X.
	Astrophys. J., 866, 100-100 (2018)
	The enigmatic compact radio source coincident with the energetic X-ray pulsar PSR J1813-1749 and HESS J1813-178.
o	Table 2: <[DRK2018] VLA JHHMMSS.ss+DDMMSS.s> N=27.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRK2021]
[DRK2021]	(Diaz+Ryan-Weber+Karman+, 2021)
Write:	<<[DRK2021] QSO J1030+0524 LAE N>>
N:	9
Object:	LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT MUSE observations of N=9 Lyman alpha emitters (LAEs) in the field of QSO J1030+0524.
Ref:	=2021MNRAS.502.2645D
by	DIAZ C.G. , RYAN-WEBER E.V., KARMAN W., CAPUTI K.I., SALVADORI S., CRIGHTON N.H., OUCHI M., VANZELLA E.
	Mon. Not. R. Astron. Soc., 502, 2645-2663 (2021)
	Faint LAEs near z > 4.7 C IV absorbers revealed by MUSE.
o	Figs 2-3, Table 2: <[DRK2021] QSO J1030+0524 LAE N> (Nos 1-8). Fig. 13, Table 3: <[DRK2021] QSO J1030+0524 LAE N> (No. 9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRL2005]
[DRL2005]	(Demarco+Rosati+Lidman+, 2005)= ([DRL2005a])
Write:	<<[DRL2005] NNNNa>>
N:	134+85
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat.	in SIMBAD: Ref. 2005A&A...432..381D is completely incorporated.
Note:	VLT FORS1 and FORS2 spectroscopic survey of the cluster RX J0152.7-1357.
in source:	RX J0152.7-1357 = ClG J0152-1357
Ref:	=2005A&A...432..381D
by	DEMARCO R. , ROSATI P., LIDMAN C., HOMEIER N.L., SCANNAPIECO E., BENITEZ N., MAINIERI V., NONINO M., GIRARDI M., STANFORD S.A., TOZZI P., BORGANI S., SILK J., SQUIRES G., BROADHURST T.J.
	Astron. Astrophys., 432, 381-394 (2005)
	A VLT spectroscopic survey of RX J0152.7-1357, a forming cluster of galaxies at z = 0.837.
o	Tables 4, 5: <[DRL2005] NNNNa> N=102+85 among (Nos 18-3019, 26b, 1238b).
Ref:	=2010ApJ...725.1252D
by	DEMARCO R. , GOBAT R., ROSATI P., LIDMAN C., RETTURA A., NONINO M., VAN DER WEL A., JEE M.J., BLAKESLEE J.P., FORD H.C., POSTMAN M.
	Astrophys. J., 725, 1252-1276 (2010)
	Star formation histories in a cluster environment at z ~ 0.84.
o	Table 1: <[DRL2005] NNNNa> N=32 among (Nos 18-5063) added.
=E=	Catalogue in electronic form as J/A+A/432/381
=E=	Catalogue in electronic form as J/ApJ/725/1252
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRL2005a]
[DRL2005a]	(Demarco+Rosati+Lidman+, 2005)
*****	Avoid the usage of [DRL2005a], prefer [DRL2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRL2005b]
[DRL2005b]	(Dannerbauer+Rigopoulou+Lutz+, 2005)
Write:	<<[DRL2005b] 06035-7102W>>
N:	2
Object:	G in Pair (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Near IR spectra of ULIRGs with SOFI on ESO NTT 3.5m telescope at La Silla. IRAS 06035-7102 has a double nuclei.
in source:	IRAS 06035-7102
Ref:	=2005A&A...441..999D
by	DANNERBAUER H. , RIGOPOULOU D., LUTZ D., GENZEL R., STURM E., MOORWOOD A.F.M.
	Astron. Astrophys., 441, 999-1010 (2005)
	Follow-up near-infrared spectroscopy of ultraluminous infrared galaxies observed by ISO.
o	Table 2: 20446-6128 is a misprint for 20446-6218.
o	Table 2: <[DRL2005b] 06035-7102W> (Nos E, W).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRL2007]
[DRL2007]	(Demarco+Rosati+Lidman+, 2007)
Write:	<<[DRL2007] NNNNNa>>
N:	38+11+189
Object:	G + (X) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT FORS, HST ACS, and Chandra observations of RDCS J1252-2927.
in source:	RDCS J1252-2927
Ref:	=2007ApJ...663..164D
by	DEMARCO R. , ROSATI P., LIDMAN C., GIRARDI M., NONINO M., RETTURA A., STRAZZULLO V., VAN DER WEL A., FORD H.C., MAINIERI V., HOLDEN B.P., STANFORD S.A., BLAKESLEE J.P., GOBAT R., POSTMAN M., TOZZI P., OVERZIER R.A., ZIRM A.W., BENITEZ N., HOMEIER N.L., ILLINGWORTH G.D., INFANTE L., JEE M.J., MEI S., MENANTEAU F., MOTTA V., ZHENG W., CLAMPIN M., HARTIG G.
	Astrophys. J., 663, 164-182 (2007)
	VLT and ACS observations of RDCS J1252.9-2927: dynamical structure and galaxy populations in a massive cluster at z = 1.237.
o	Tables 2,3,4,5: <[DRL2007] NNNNNa> N=38+11+189 among (Nos 1-60005, 2545b).
=E=	Catalogue in electronic form as J/ApJ/663/164
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRM2013]
[DRM2013]	(Dunlop+Rogers+McLure+, 2013)
Write:	<<[DRM2013] UDFParN-SSss-MSSs>>
N:	25
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=24 galaxies found in the WFC3 infrared imaging from the Hubble Space Telescope (HST) Ultra-Deep Field UDF09 parallel fields (UDF09P1 and UDF09P2). Regarding the partial coordinates in the format '-SSss-MSSs': the complete 2000 coordinate format is 03 32 SS.ss (right ascension) and -27 4M SS.s (declination). See also [MDB2013].
Ref:	=2013MNRAS.432.3520D
by	DUNLOP J.S. , ROGERS A.B., McLURE R.J., ELLIS R.S., ROBERTSON B.E., KOEKEMOER A., DAYAL P., CURTIS-LAKE E., WILD V., CHARLOT S., BOWLER R.A.A., SCHENKER M.A., OUCHI M., ONO Y., CIRASUOLO M., FURLANETTO S.R., STARK D.P., TARGETT T.A., SCHNEIDER E.
	Mon. Not. R. Astron. Soc., 432, 3520-3533 (2013)
	The UV continua and inferred stellar populations of galaxies at z ≃ 7-9 revealed by the Hubble ultra-deep field 2012 campaign.
o	Table A1: <[DRM2013] UDFParN-SSss-MSSs> N=25.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRM99]
[DRM99]	(Drissen+Roy+Moffat+, 1999)
Write:	<<[DRM99] NGC 2403 R>> <<[DRM99] NGC 2403 R-NN>> <<[DRM99] NGC 2403 I A>> <<[DRM99] NGC 2403 I EMN>> <<[DRM99] NGC 2403 IV A>> <<[DRM99] 4-NN>> <<[DRM99] 5-NN>>
N:	6+50+4+5+1+52+25
Object:	Poss. WR + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST WFPC2 and CFHT observations. Table 1: N=6 giant HII regions in NGC 2403, format 'NGC 2403 R'. Table 2: WR candidates in the HII regions, format 'NGC 2403 R NN', NGC 2403 I: N=22, NGC 2403 II: N=11, NGC 2403 IV: N=9, NGC 2403 V: N=6, NGC 2403 VI: N=2. (NGC 2403 III is not observed). Fig.6: N=4 subclusters of stars, (Nos A-D), in NGC 2403 I. Fig.8: N=5 Em., (Nos EM1-EM5), in NGC 2403 I. Fig.16b: N=1 compact Cl, (No. A), in NGC 2403 IV. Table 4: N=52 WR* candidates in the field of NGC 2403, format '4-NN'. Table 5: N=25 G or Cl* in the field of NGC 2403, format '5-NN'.
in source:	NGC 2403
Ref:	=1999AJ....117.1249D
by	DRISSEN L. , ROY J.-R., MOFFAT A.F.J., SHARA M.M.
	Astron. J., 117, 1249-1274 (1999)
	The ionizing star clusters of giant H II regions in NGC 2403.
o	Table 1: <[DRM99] NGC 2403 R> (Nos I-VI). Table 2: <[DRM99] NGC 2403 R-NN> N=50. Fig.6: <[DRM99] NGC 2403 I A> (Nos A-D). Fig.8: <[DRM99] NGC 2403 I EMN> (Nos EM1-EM5). Fig.16b: <[DRM99] NGC 2403 IV A> (No. A). Table 4: <[DRM99] 4-NN> (Nos 4-1 to 4-52). Table 5: <[DRM99] 5-NN> (Nos 5-1 to 5-25).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DROXO
DROXO	(Deep Rho Ophiuchi XMM-Newton Observation)
Write:	<<DROXO NNN>>
N:	111
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of the Rho Ophiuchi Cloud.
in source:	NAME rho Oph Cloud
Ref:	=2010A&A...519A..34P
by	PILLITTERI I. , SCIORTINO S., FLACCOMIO E., STELZER B., MICELA G., DAMIANI F., TESTI L., MONTMERLE T., GROSSO N., FAVATA F., GIARDINO G.
	Astron. Astrophys., 519A, 34-34 (2010)
	Results from DROXO. III. Observation, source list, and X-ray properties of sources detected in the ``Deep ρ Ophiuchi XMM-Newton observation''.
o	Table A.1: <DROXO NNN> (Nos 1-111).
=E=	Catalogue in electronic form as J/A+A/519/A34
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DRP
DRP	(D. Reverte-Payo)
*****	Avoid the usage of DRP, prefer [RVH2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DRP2007]
[DRP2007]	(Donley+Rieke+Perez-Gonzalez+, 2007)
Write:	<<[DRP2007] NNNNN>>
N:	62
Object:	G (SIMBAD class: AGN_Candidate = Active Galaxy Nucleus Candidate)
Note:	Spitzer IRAC and MIPS observations of the CDFN.
in source:	NAME CDFN
Ref:	=2007ApJ...660..167D
by	DONLEY J.L. , RIEKE G.H., PEREZ-GONZALEZ P.G., RIGBY J.R., ALONSO-HERRERO A.
	Astrophys. J., 660, 167-190 (2007)
	Spitzer power-law active galactic nucleus candidates in the Chandra Deep Field-North.
o	Table 1: <[DRP2007] NNNNN> N=62 among (Nos 8962-54888).
=E=	Catalogue in electronic form as J/ApJ/660/167
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRR2000]
[DRR2000]	(Drissen+Roy+Robert+, 2000)
Write:	<<[DRR2000] Cluster A>> <<[DRR2000] Star N>> <<[DRR2000] WRN>> <<[DRR2000] NGC 2366 BGNN>>
N:	2+2+4+14
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST FOS, WFPC2, STIS, and CFHT MONICA observations. Figs 6, 7: in the field of NGC 2363: N=2 clusters of stars, Cluster A = [GPT94] Knot A, and Cluster B contains [GPT94] Knot B. N=2 stellar objects, 'Star 1' and 'Star 2'. N=4 WR* candidates, in Cluster B, (Nos WR1-WR4). Table 1: in the field on NGC 2366: N=14 Background galaxies (BG in the format). See also [GPT94].
in source:	NGC 2363
in source:	NGC 2366
Ref:	=2000AJ....119..688D
by	DRISSEN L. , ROY J.-R., ROBERT C., DEVOST D., DOYON R.
	Astron. J., 119, 688-704 (2000)
	The star formation history of the starburst region NGC 2363 and its surroundings.
o	Fig.1: HII regions = [M94c] NGC 2366 1 to 3.
o	Figs 6, 7: <[DRR2000] Cluster A> (Nos A-B), <[DRR2000] Star N> (Nos 1-2), <[DRR2000] WRN> (Nos WR1-WR4). Table 1: <[DRR2000] NGC 2366 BGNN> (Nos BG1 to BG14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRR2005]
[DRR2005]	(Donley+Rieke+Rigby+, 2005)
Write:	<<[DRR2005] JHHMMSS.ss+DDMMSS.s>>
N:	16+11
Object:	AGN (SIMBAD class: AGN = Active Galaxy Nucleus)
Stat:	is completely incorporated in Simbad
Note:	Chandra, Spitzer MIPS and VLA observations. Sample of 27 radio-excess AGNs in the Chandra CDFN. Initial sample from [R2000].
in source:	NAME CDFN
Ref:	=2005ApJ...634..169D
by	DONLEY J.L. , RIEKE G.H., RIGBY J.R., PEREZ-GONZALEZ P.G.
	Astrophys. J., 634, 169-182 (2005)
	Unveiling a population of AGNs not detected in X-rays.
o	Table 1: <[DRR2005] JHHMMSS.ss+DDMMSS.s> N=16+11.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRR2009]
[DRR2009]	(Davis+Richer+Rich+, 2009)= (WD) = (GemWD)
Write:	<<[DRR2009] LRIS-NN>> <<[DRR2009] GMOS-NN>>
N:	30+20
Object:	WD (SIMBAD class: WhiteDwarf = White Dwarf)
Note:	Keck LRIS and Gemini GMOS observations of white dwarfs in the direction of the globular cluster Messier 4.
in source:	M 4 = NGC 6121
Ref:	=2009ApJ...705..398D
by	DAVIS D.S. , RICHER H.B., RICH R.M., REITZEL D.R., KALIRAI J.S.
	Astrophys. J., 705, 398-407 (2009)
	The spectral types of white dwarfs in Messier 4.
o	Table 1, col(1): <[DRR2009] LRIS-NN> N=23 among (Nos 0-29) = Table 1, col(2): <[DRR2009] GMOS-NN> N=18 among (Nos 1-21).
Ref:	=2009ApJ...705..408K
by	KALIRAI J.S. , DAVIS D.S., RICHER H.B., BERGERON P., CATELAN M., HANSEN B.M.S., RICH R.M.
	Astrophys. J., 705, 408-425 (2009)
	The masses of population II white dwarfs.
o	Table 1: <[DRR2009] LRIS-NN> (Nos 0-30), <[DRR2009] GMOS-NN> (Nos 5, 17) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRR96]
[DRR96]	(Drissen+Roy+Robert, 1996)
Write:	<<[DRR96] NGC 2363 VN>>
N:	1
Object:	Blue V* (SIMBAD class: Variable* = Variable Star)
in source:	NGC 2363
Ref:	=1996IAUC.6294....1D
by	DRISSEN L. , ROY J.-R., ROBERT C.
	IAU Circ., 6294, 1-None (1996)
	NGC 2363.
o	<[DRR96] NGC 2363 VN> (No. V1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRS2009]
[DRS2009]	(Da Rio+Robberto+Soderblom+Panagia+, 2009)
Write:	<<[DRS2009] NNNN>>
N:	2621
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	ESO/MPI 2.2m telescope WFI photometry of the Orion Nebula Cluster.
in source:	NAME ONC
Ref:	=2009ApJS..183..261D
by	DA RIO N. , ROBBERTO M., SODERBLOM D.R., PANAGIA N., HILLENBRAND L.A., PALLA F., STASSUN K.
	Astrophys. J., Suppl. Ser., 183, 261-277 (2009)
	A multi-color optical survey of the Orion nebula cluster. I. The catalog.
o	Table 2: <[DRS2009] NNNN> (Nos 1-2621).
=E=	Catalogue in electronic form as J/ApJS/183/261
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DRT03
DRT03	(De Buizer+Radomski+Telesco+, 2003)
====>	Equivalent to: [DRT2003]
Origin	of the Acronym: L (2005ApJS..156..179D)
Details on Acronym: DRT05
DRT05	(De Buizer+Radomski+Telesco+, 2005)
Write:	<<DRT05 GLL.ll+B.bb N>> <<DRT05 Cep A HW 2 N>>
N:	29
Object:	(Mid IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	NASA IRTF observations. Mid-IR images of 29 sources in 15 sites of water masers See also DPT00 and [DRT2003].
Ref:	=2005ApJS..156..179D
by	DE BUIZER J.M. , RADOMSKI J.T., TELESCO C.M., PINA R.K.
	Astrophys. J., Suppl. Ser., 156, 179-215 (2005)
	Observations of massive star-forming regions with water masers: mid-infrared imaging.
o	Table 2: <DRT05 GLL.ll+B.bb N> N=28, <DRT05 Cep A HW 2 N> N=1.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DRT2000]
[DRT2000]	(De la Varga+Reimers+Tytler+, 2000)
Write:	<<[DRT2000] QSO JHHMM+DDMM abs N.NN>> <<[DRT2000] QSO JHHMM+DDMM abs N.NNNN>>
N:	20
Object:	DLA
Note:	DLAs in the line of sight of 21 QSOs.
Ref:	=2000A&A...363...69D
by	DE LA VARGA A. , REIMERS D., TYTLER D., BARLOW T., BURLES S.
	Astron. Astrophys., 363, 69-83 (2000)
	Damped Lymanα systems at z=0.68 and z=1.15 towards HE 1122-1649 and HE 0515-4414.
o	Tables 7, 8 are considered as a compilation: no other acronyms are given for DLAs already cited in previous references.
o	Tables 7, 8: <[DRT2000] QSO JHHMM+DDMM abs N.NN>, <[DRT2000] QSO JHHMM+DDMM abs N.NNNN>, N=20.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRT2003]
[DRT2003]	(De Buizer+Radomski+Telesco+, 2003)= (DOC05) = (DRT03)
Write:	<<[DRT2003] GLL.ll+B.bb N>>
N:	9+7+6+5+7
Object:	(Mid IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	NASA IRTF observations. Mid-IR images of 30 sources in 5 fields (HII regions [HC96]). See also DPT00 and DRT05.
in source:	[HC96] G09.62+0.19
in source:	[HC96] G11.94-0.62
in source:	[HC96] G19.61-0.23
in source:	[HC96] G34.26+0.15
in source:	[HC96] G45.07+0.13
Ref:	=2003ApJ...598.1127D
by	DE BUIZER J.M. , RADOMSKI J.T., TELESCO C.M., PINA R.K.
	Astrophys. J., 598, 1127-1139 (2003)
	A search for mid-infrared emission from hot molecular core candidates.
o	Table 2: <[DRT2003] GLL.ll+B.bb N> N=30.
Ref:	=2005ApJ...635..452D
by	DE BUIZER J.M. , OSORIO M., CALVET N.
	Astrophys. J., 635, 452-465 (2005)
	Observations and modeling of the 2-25 µm emission from high-mass protostellar object candidates.
o	Fig.3, Table 4: <[DRT2003] G45.07+0.13 N> (Nos 4-7) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRV2022]
[DRV2022]	(Daddi+Rich+Valentino+, 2022)
Write:	<<[DRV2022] FVX-LAB>> <<[DRV2022] RO-HHMM>>
N:	1+2
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Keck KCWI observations of N=1 Lymanα blob (LAB) and N=2 radio overdensities (RO).
Ref:	=2022ApJ...926L..21D
by	DADDI E. , RICH R.M., VALENTINO F., JIN S., DELVECCHIO I., LIU D., STRAZZULLO V., NEILL J., GOBAT R., FINOGUENOV A., BOURNAUD F., ELBAZ D., KALITA B.S., O'SULLIVAN D., WANG T.
	Astrophys. J., 926L, 21-21 (2022)
	Evidence for Cold-stream to Hot-accretion Transition as Traced by Lyα Emission from Groups and Clusters at 2 < z < 3.3.
o	Fig. 1, Table 1: <[DRV2022] FXV-LAB> N=1, <[DRV2022] RO-HHMM> (Nos RO-0958, RO-0959).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DRW83]
[DRW83]	(D'Odorico+Rosa+Wampler, 1983)
Write:	<<[DRW83] NGC 300 NN>> <<[DRW83] He 2-10 N>> <<[DRW83] NGC 604 A>>
N:	15+3+7
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	HII regions in NGC 300, He 2-10, and NGC 604. Some of the HII regions seems to be WR clusters.
in source:	NGC 300
in source:	Hen 2-10
in source:	NGC 604
Ref:	=1983A&AS...53...97D
by	D'ODORICO S. , ROSA M., WAMPLER E.J.
	Astron. Astrophys., Suppl. Ser., 53, 97-108 (1983)
	Search for Wolf-Rayet features in the spectra of giant HII regions. I. Observations in NGC 300, NGC 604, NGC 5457 and He 2-10.
o	Table III: <[DRW83] NGC 300 NN> (Nos 1-15), <[DRW83] He 2-10 N> (Nos 1-3). Table IV: <[DRW83] NGC 604 A> (Nos A-G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DS
DS	(Dressler+Shectman)
*****	Avoid the usage of DS, prefer [DS88]
Origin	of the Acronym: L (2001AJ....122.1289T)
Details on Acronym: DS
DS	(Deep Survey)
*****	Avoid the usage of DS, prefer EDS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DS
DS	(Drilling S.)
Write:	<<PN DS N>>
N:	2
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	The central * of DS 1 is LSS 2018. The central * of DS 2 is LSS 125 = PN G335.5+12.4 = PK 335+12 1
Ref:	=1983ApJ...270L..13D
by	DRILLING J.S.
	Astrophys. J., 270, 13-15 (1983)
	The spectra of 12 new subluminous O stars.
o	Table 1: <LSE NNN> N=7 among (Nos 21-263) added. Not numbered i,n the paper: <PN DS N> (Nos 1-2).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [DS2008]
[DS2008]	(Danforth+Shull, 2008) (Not yet in Simbad)
Write:	<<[DS2008] QSO JHHMM+DDMM abs N.NNNNN>>
N:	650
Object:	Absorber
Note:	HST and FUSE spectroscopic survey.
Ref:	=2008ApJ...679..194D
by	DANFORTH C.W. , SHULL J.M.
	Astrophys. J., 679, 194-219 (2008)
	The low-z intergalactic medium. III. H I and metal absorbers at z < 0.4.
o	In tables HE 0226-4410 is a misprint for HE 0226-4110
o	Tables 2, 4: <[DS2008] QSO JHHMM+DDMM abs N.NNNNN> N=650.
=E=	Catalogue in electronic form as <J/ApJ/679/194/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DS77]
[DS77]	(Dyck+Simon, 1977)= (IRS)
Write:	<<[DS77] W 33 IRS N>>
N:	3
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	W 33
Ref:	=1977ApJ...211..421D
by	DYCK H.M. , SIMON T.
	Astrophys. J., 211, 421-428 (1977)
	Infrared observations of compact H II regions in the spectral range 3.4-33 micrometers.
o	IRS in W 51 and W 75 = '[WBN74] W 51 IRS N' and [WBN74] W 75 IRS N'
o	Table 1: <[WBN72] W 3 IRS NN> (No. 10) added. Table 1: <[DS77] W 33 IRS N> (Nos 1-3). Table 2: <NAME DR 21 IRS>, <NAME DR 21 (N and S)>, <NAME W 75 (N)>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DS84]
[DS84]	(Dickey+Salpeter, 1984)
Write:	<<[DS84] NN>>
N:	66
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
in source:	ACO 2151
Ref:	=1984ApJ...284..461D
by	DICKEY J.M. , SALPETER E.E.
	Astrophys. J., 284, 461-470 (1984)
	1.4 GHz continuum sources in the Hercules cluster.
o	Table 1: <[DS84] NN> (Nos 1-66)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DS88]
[DS88]	(Dressler+Shectman, 1988)= (DS)
Write:	<<[DS88] ACO NNNN NNN>> <<[DS88] DRCG HHMM+DD NNN>>
N:	2100
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	N=2100 galaxies in 14 'ACO' and 'DRCG' clusters. See also [D80].
Ref:	=1988AJ.....95..284D
by	DRESSLER A. , SHECTMAN S.A.
	Astron. J., 95, 284-297 (1988)
	A catalog of 1268 radial velocities in 15 rich clusters.
o	Catalog for 14 clusters (not 15).
o	Table I: <[DS88] ACO NNNN NNN>, <[DS88] DRCG HHMM-DD NNN>, N=2100.
=E=	Catalogue in electronic form as J/AJ/95/284
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DS89]
[DS89]	(Downes+Szkody, 1989)
Write:	<<[DS89] AA CCC NN>> <<[DS89] CCC YYYY NN>>
N:	79
Object:	* (SIMBAD class: Star)
Note:	Tables III to IX: * in the fields of novae 'AA CCC': T Boo, AB Boo, SY Gem, VZ Gem, U Leo, and in the fields of novae 'CCC YYYY': Gem 1892 and Leo 1612. Maps in Fig. 1-6, 9
Ref:	=1989AJ.....97.1729D
by	DOWNES R.A. , SZKODY P.
	Astron. J., 97, 1729-1736 (1989)
	CCD observations of old nova fields.
o	<[DS89] AA CCC NN>, <[DS89] CCC YYYY NN>, N=79
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DS93]
[DS93]	(Downes+Shara, 1997)
*****	Avoid the usage of [DS93], prefer [DWS97]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DS95]
[DS95]	(Danilov+Seleznev, 1995)= (GSC)
Write:	<<[DS95] NN>>
N:	11
Object:	Star-Gas complex (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Ref:	=1995AZh....72..333D
by	DANILOV V.M. , SELEZNEV A.F.
	Astron. Zh., 72, 333-343 (1995)
	Estimates of geometric and dynamic parameters of star-gas complexes in the Galaxy.
o	Tables 1, 2: <[DS95] NN> (Nos 1-11)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DS96]
[DS96]	(Davis+Smith, 1996)
Write:	<<[DS96] AN>> <<[DS96] Knot A>>
N:	6+3+26
Object:	(IR) + * + Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=6 IR sources (Nos I1-I6). N=3 reference stars (Nos O1-O3). No. O3 is added in the 2nd ref. N=26 knots, (Nos A-M) are in the eastern lobe of DR 21, (Nos N-Z) are in the western lobe of DR 21. Map. See also [ICB99].
in source:	DR 21
Ref:	=1996A&A...310..961D
by	DAVIS C.J. , SMITH M.D.
	Astron. Astrophys., 310, 961-969 (1996)
	Near-IR imaging and spectroscopy of DR21: a case for supersonic turbulence.
o	Table 1: <[DS96] IN> (Nos I1-I6), <[DS96] ON> (Nos O1-O2). Fig.4: <[DS96] Knot A> (Nos A-Z).
Ref:	=1999MNRAS.304..406I
by	ITOH Y. , CHRYSOSTOMOU A., BURTON M., HOUGH J.H., TAMURA M.
	Mon. Not. R. Astron. Soc., 304, 406-414 (1999)
	The magnetic field structure of the DR 21 region.
o	Fig.1: <[DS96] O3> added. Table 2: <[ICB99] WN> (Nos E1-E5, W1-W5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DS98]
[DS98]	(Dumm+Schild, 1998)
Write:	<<[DS98] NNN>>
N:	350
Object:	M Giant (SIMBAD class: Star)
Ref:	=1998NewA....3..137D
by	DUMM T. , SCHILD H.
	New Astronomy, 3, 137-156 (1998)
	Stellar radii of M giants.
o	<[DS98] NNN> (Nos 1-350).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSA2001]
[DSA2001]	(Decourchelle+Sauvageot+Audard+, 2001) (Not yet in Simbad)
Write:	<<[DSA2001] AN>> <<[DSA2001] A>>
N:	3+2
Object:	Knot (SIMBAD class: Region = Region defined in the Sky)
Note:	N=3 SE knots in Thycho SNR, (Nos C1-C3), Map Fig.3. N=2 regions, A is red, B is blue. Map Fig.5.
in source:	NAME Tycho SNR
Ref:	=2001A&A...365L.218D
by	DECOURCHELLE A. , SAUVAGEOT J.L., AUDARD M., ASCHENBACH B., SEMBAY S., ROTHENFLUG R., BALLET J., STADLBAUER T., WEST R.G.
	Astron. Astrophys., 365, 218-224 (2001)
	XMM-Newton observation of the Tycho supernova remnant.
o	Table 1: <[DSA2001] AN> (Nos C1-C3), <[DSA2001] A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSB2001]
[DSB2001]	(Dawson+Stern+Bunker+, 2001)
Write:	<<[DSB2001] FMMSSs-MMSS>>
N:	49
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=49 seredipitous detected G outside of the central HDF. 5 are members of ClG J1236+6215. Format 'FMMSSs-MMSS', offset relative to RA: 12h, Dec: +62deg.
in source:	NAME HDFN
Ref:	=2001AJ....122..598D
by	DAWSON S. , STERN D., BUNKER A.J., SPINRAD H., DEY A.
	Astron. J., 122, 598-610 (2001)
	Serendipitously detected galaxies in the Hubble Deep Field.
o	Table 2: <[DSB2001] FMMSSs-MMSS> N=49.
=E=	Catalogue in electronic form as J/AJ/122/598
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSB2004]
[DSB2004]	(De Grijs+Smith+Bunker+, 2004)
Write:	<<[DSB2004] NN>>
N:	15 among 19
Object:	Poss. Star Cluster (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	H band spectroscopy of NGC 1140 from the Gemini-South telescope equipped with CIRPASS, to search for young massive star clusters (YMC). Among the 15 objects observed, 8 are identified as YMC.
in source:	NGC 1140
Ref:	=2004MNRAS.352..263D
by	DE GRIJS R. , SMITH L.J., BUNKER A., SHARP R.G., GALLAGHER III J.S., ANDERS P., LANCON A., O'CONNELL R.W., PARRY I.R.
	Mon. Not. R. Astron. Soc., 352, 263-276 (2004)
	CIRPASS near-infrared integral-field spectroscopy of massive star clusters in the starburst galaxy NGC 1140.
o	Fig.1, Table 2: <[DSB2004] NN> (Nos 1-9, 14-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSB2008]
[DSB2008]	(Deharveng+Small+Barlow+, 2008)
Write:	<<[DSB2008] NNNNN>>
N:	96
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	GALEX spectroscopic search for Ly-alpha-emitting galaxies.
Ref:	=2008ApJ...680.1072D
by	DEHARVENG J.-M. , SMALL T., BARLOW T.A., PEROUX C., MILLIARD B., FRIEDMAN P.G., MARTIN D.C., MORRISSEY P., SCHIMINOVICH D., FORSTER K., SEIBERT M., WYDER T.K., BIANCHI L., DONAS J., HECKMAN T.M., LEE Y.-W., MADORE B.F., NEFF S.G., RICH R.M., SZALAY A.S., WELSH B.Y., YI S.K.
	Astrophys. J., 680, 1072-1082 (2008)
	Lyα-emitting galaxies at 0.2<z<0.35 from GALEX spectroscopy.
o	Table 2, col(2): <[DSB2008] NNNNN> N=96 among (Nos 958-37457).
=E=	Catalogue in electronic form as J/ApJ/680/1072
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSB2018]
[DSB2018]	(Diego+Schmidt+Broadhurst+, 2018)
Write:	<<[DSB2018] A370 NN>> <<[DSB2018] A370 NN.N>> <<[DSB2018] A370 NN.N.NN>>
N:	30+91+149
Object:	Grav. lensed image + Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=30 multiply imaged systems (format A370 NN) in the field of the galaxy cluster ACO 370, N=91 gravitationally lensed images (format A370 NN.N) in those systems, and N=149 multiply imaged knots (format A370 NN.N.NN). Use of publicly available HST Frontier Fields, GLASS, and Chandra data.
in source:	ACO 370
Ref:	=2018MNRAS.473.4279D
by	DIEGO J.M. , SCHMIDT K.B., BROADHURST T., LAM D., VEGA-FERRERO J., ZHENG W., LEE S., MORISHITA T., BERNSTEIN G., LIM J., SILK J., FORD H.
	Mon. Not. R. Astron. Soc., 473, 4279-4296 (2018)
	A free-form lensing model of A370 revealing stellar mass dominated BCGs, in Hubble Frontier Fields images.
o	Fig. 6, Table A1: <[DSB2018] A370 NN> (Nos 1-30), <[DSB2018] A370 NN.N> N=91, <[DSB2018] A370 NN.N.NN> N=149.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSB94]
[DSB94]	(Deharveng+Sasseen+Buat+, 1994)= (FAUST)
Write:	<<[DSB94] NNN>>
N:	142 among 320
Object:	G (SIMBAD class: Galaxy)
Note:	Observations of the FAUST telescope on Atlas 1
Ref:	=1994A&A...289..715D
by	DEHARVENG J.-M. , SASSEEN T.P., BUAT V., BOWYER S., LAMPTON M., WU X.
	Astron. Astrophys., 289, 715-728 (1994)
	Ultraviolet observations of galaxies with the FAUST experiment.
o	<[DSB94] NNN> N=142 among 320
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSC2002]
[DSC2002]	(Dolphin+Saha+Claver+, 2002)
Write:	<<[DSC2002] CN-VNN>>
N:	10+82
Object:	V* (SIMBAD class: Variable* = Variable Star)
in source:	NAME Leo A
Ref:	=2002AJ....123.3154D
by	DOLPHIN A.E. , SAHA A., CLAVER J., SKILLMAN E.D., COLE A.A., GALLAGHER J.S., TOLSTOY E., DOHM-PALMER R.C., MATEO M.
	Astron. J., 123, 3154-3198 (2002)
	Variable stars in Leo A: RR Lyrae stars, short-period cepheids, and implications for stellar content.
o	Tables 2 and 3 : x-y coordinates; objects not in Simbad.
o	Table 3: <[DSC2002] CN-VNN> N=10+82.
=E=	Catalogue in electronic form as J/AJ/123/3154
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSC2003]
[DSC2003]	(De filippis+Schindler+Castillo-Morales, 2003)
Write:	<<[DSC2003] NN>> <<[DSC2003] MN>>
N:	19+2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM observations of ClG 0939+4713.
in source:	ClG 0939+4713 = ACO 851
Ref:	=2003A&A...404...63D
by	DE FILIPPIS E. , SCHINDLER S., CASTILLO-MORALES A.
	Astron. Astrophys., 404, 63-74 (2003)
	XMM observation of the dynamically young galaxy cluster CL 0939+4713.
o	Table 1: <[DSC2003] MN> (Nos M1-M2). Table 2: <[DSC2003] NN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSC2005]
[DSC2005]	(Dietrich+Schneider+Clowe+, 2005)
Write:	<<[DSC2005] A223-W>> <<[DSC2005] WW peak>> <<[DSC2005] arclet N>>
N:	2+1+2
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Weak lensing analysis of the double cluster ACO 222 and ACO 223: ACO 223 shows two distinct peaks separated by about 4' in the galaxy distribution and X-ray emission. A223-N and A223-S. A new cluster is seen SE of ACO 222, designated as SE peak of galaxies. Two arclets are found in ACO 222.
in source:	ACO 222
in source:	ACO 223
Ref:	=2005A&A...440..453D
by	DIETRICH J.P. , SCHNEIDER P., CLOWE D., ROMANO-DIAZ E., KERP J.
	Astron. Astrophys., 440, 453-471 (2005)
	Weak lensing study of dark matter filaments and application to the binary cluster A 222 and A 223.
o	Text: <[DSC2005] A223-W> (Nos S, N). Text: <[DSC2005] SE peak> N=1. Table A1: <[DSC2005] arclet N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSC97]
[DSC97]	(Duncan+Stewart+Campbell-Wilson+, 1997)
Write:	<<[DSC97] JHHMM-DDMM>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Objects around SNR 272.2-03.2. Fig. 2: Map
Ref:	=1997MNRAS.289...97D
by	DUNCAN A.R. , STEWART R.T., CAMPBELL-WILSON D., HAYNES R.F., ASCHENBACH B., JONES K.L.
	Mon. Not. R. Astron. Soc., 289, 97-104 (1997)
	Radio observations of the X-ray supernova remnant G272.2-3.2.
o	Table 2: <[DSC97] JHHMM-DDMM> N=3
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSD2009]
[DSD2009]	(Desai+Soifer+Dey+, 2009)
Write:	<<[DSD2009] SST24 JHHMMSS.s+DDMMSS.s>>
N:	23
Object:	ULIRG (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRS observations of N=23 high-redshift ULIRGs in the Bootes field of the NOAO Deep Wide-Field Survey.
in source:	NAME Bootes Field
Ref:	=2009ApJ...700.1190D
by	DESAI V. , SOIFER B.T., DEY A., LE FLOC'H E., ARMUS L., BRAND K., BROWN M.J.I., BRODWIN M., JANNUZI B.T., HOUCK J.R., WEEDMAN D.W., ASHBY M.L.N., GONZALEZ A., HUANG J., SMITH H.A., TEPLITZ H., WILLNER S.P., MELBOURNE J.
	Astrophys. J., 700, 1190-1204 (2009)
	Strong polycyclic aromatic hydrocarbon emission from z ~ 2 ULIRGs.
o	Tables 1-3: <[DSD2009] SST4 JHHMMSS.s+DDMMSS.s> N=23.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSD2020]
[DSD2020]	(Sun+Deliyannis+Steinhauer+, 2020)
Write:	<<[DSD2020] NNNN>>
N:	287
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	WIYN 3.5m telescope spectroscopic observations of N=287 stars in NGC 2548, as part of the WIYN open cluster study (WOCS).
in source:	NGC 2548 = M 48
Ref:	=2020AJ....159..220S
by	SUN Q. , DELIYANNIS C.P., STEINHAUER A., TWAROG B.A., ANTHONY-TWAROG B.J.
	Astron. J., 159, 220-220 (2020)
	WIYN open cluster study LXXIX. M48 (NGC 2548) I. Radial velocities, rotational velocities, and metallicities of stars in the open cluster M48 (NGC 2548).
o	Table 3 : <[DSD2020] NNNN> N=287 among (Nos 2001-2373).
=E=	Catalogue in electronic form as <J/AJ/159/220/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSD94]
[DSD94]	(Drissen+Shara+Dopita+, 1994)
Write:	<<[DSD94] VHHMM+DDMM>>
N:	7
Object:	V* (SIMBAD class: CataclyV* = Cataclysmic Binary)
Stat:	is completely incorporated in Simbad
Note:	In the format the letter 'V' is for Variable star, the coordinates are (2000)
Ref:	=1994AJ....107.2172D
by	DRISSEN L. , SHARA M.M., DOPITA M., WICKRAMASINGHE D.T.
	Astron. J., 107, 2172-2178 (1994)
	A survey for highly variable objects on the SRC-J plates. I. Faint new cataclysmic variables in the galactic halo.
o	<[DSD94] VHHMM-DDMM> N=7
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSD95]
[DSD95]	(Dey+Spinrad+Dickinson, 1995)
Write:	<<[DSD95] J1019+0535 A>>
N:	4
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck observations. Image of MITG J1019+0535 field: (Nos A-D). A is associated with the radio-source. A and B may or may not be physically related. D is an extremely red object.
Ref:	=1995ApJ...440..515D
by	DEY A. , SPINRAD H., DICKINSON M.
	Astrophys. J., 440, 515-524 (1995)
	Discovery of a z = 2.76 dusty radio galaxy.
o	Table 1, Fig.2: <[DSD95] J1019+0535 A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSE2005]
[DSE2005]	(De Filippis+Schindler+, 2005)
Write:	<<[DSE2005] BNN>>
N:	14
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	RASS archives are used to detect new X-ray cluster candidates. 14 are new. Optical follow-up observations with WIFI on ESO 2.2m telescope.
in source:	NAME Shapley Concentration = NAME Shapley Supercluster
Ref:	=2005A&A...444..387D
by	DE FILIPPIS E. , SCHINDLER S., ERBEN T.
	Astron. Astrophys., 444, 387-402 (2005)
	The Shapley super-cluster. New X-ray detections and mass distribution.
o	Table 4: <[DSE2005] BNN> (Nos B1-B14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSF2003]
[DSF2003]	(Doi+Supernova Cosmology Project+Fadeyev+, 2003)
Write:	<<[DSF2003] JHHMMSS.ss+DDMMSS.s>>
N:	12
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Subaru observations. Host galaxies of SN 2002KM and SN 2002KO to SN 2002KY.
Ref:	=2003IAUC.8119....1D
by	DOI M. , (The Supernova Cosmology Project), FADEYEV V., LEE B., STANISHEV V., VOGEL R., YASUDA N., KASHIKAWA N., MOTOHARA K., MOROKUMA T., SEKIGUCHI K., KOSUGI G., FURUSAWA H., KOMIYAMA Y., TAKATA T., OUCHI M., OHYAMA Y.
	IAU Circ., 8119, 1-None (2003)
	Supernovae 2002km-2002ky.
o	<[DSF2003] JHHMMSS.ss+DDMMSS.s> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSF2018]
[DSF2018]	(Da Costa+Soria+Farrell+, 2018)
Write:	<<[DSF2018] SMSS J1305-2931 WW blob>>
N:	2
Object:	Blob (SIMBAD class: EmObj = Emission Object)
Stat:	is completely incorporated in Simbad
Note:	2m Faulkes South Telescope observations of N=2 diffuse blobs symmetrically located on either side of the star SMSS J130522.47-293113.0.
Ref:	=2018MNRAS.477..766D
by	DA COSTA G.S. , SORIA R., FARRELL S.A., BAYLISS D., BESSELL M.S., VOGT F.P.A., ZHOU G., POINTS S.D., BEERS T.C., LOPEZ-SANCHEZ A.R., BANNISTER K.W., BELL M., HANCOCK P.J., BURLON D., GAENSLER B.M., SADLER E.M., TINGAY S., KELLER S.C., SCHMIDT B.P., TISSERAND P.
	Mon. Not. R. Astron. Soc., 477, 766-779 (2018)
	SMSS J130522.47-293113.0: a high-latitude stellar X-ray source with pc-scale outflow relics?
o	Fig. 2, Table 2: <[DSF2018] SMSS J1305-2931 WW blob> (Nos NE, SW).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSF2019]
[DSF2019]	(Dunham+Sharon+Florian+, 2019)
Write:	<<[DSF2019] SGAS J1438 Image N>> <<[DSF2019] SGAS J1438 NN.N>>
N:	4+38
Object:	Grav. lensed image of a G + Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST ACS and WFC3 observations of N=4 gravitational lensed images of luminous infrared galaxy SGAS J143845.1+145407, and N=38 gravitational lensed images of emission knots. See also [GRS2013b].
Ref:	=2019ApJ...875...18D
by	DUNHAM S.J. , SHARON K., FLORIAN M.K., RIGBY J.R., GLADDERS M.D., BAYLISS M.B., DAHLE H., JOHNSON T.L., MURRAY K., WHITAKER K.E., WUYTS E.
	Astrophys. J., 875, 18-18 (2019)
	Lens model and source reconstruction reveal the morphology and star formation distribution in the cool spiral LIRG SGAS J143845.1+145407.
o	Fig. 2: <[DSF2019] SGAS J1438 Image N> (Nos 1-4). Fig. 3, Table 1: <[DSF2019] SGAS J1438 NN.N> N=38 among (Nos 10.1-10.3 to 23.1-23.4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSG2004]
[DSG2004]	(Dickinson+Stern+Giavalisco+, 2004)
Write:	<<[DSG2004] SiD NN>> <<[DSG2004] NiD NNN>>
N:	96+155
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	GOODS (Great Observatories Origins Deep Survey) color-selected high redshift galaxy candidates from three-epoch co-added ACS mosaics. N=96 in the GOODS South Field, and N=155 in the GOODS North Field.
in source:	NAME GOODS North Field
in source:	NAME GOODS South Field
Ref:	=2004ApJ...600L..99D
by	DICKINSON M. , STERN D., GIAVALISCO M., FERGUSON H.C., TSVETANOV Z., CHORNOCK R., CRISTIANI S., DAWSON S., DEY A., FILIPPENKO A.V., MOUSTAKAS L.A., NONINO M., PAPOVICH C., RAVINDRANATH S., RIESS A., ROSATI P., SPINRAD H., VANZELLA E.
	Astrophys. J., 600, 99-102 (2004)
	Color-selected galaxies at z ~ 6 in the Great Observatories Origins Deep Survey.
o	Table 1: <[DSG2004] SiD NN> (Nos 1-96), <[DSG2004] NiD NNN> (Nos 1-155).
=E=	Catalogue in electronic form as J/ApJ/600/L99
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSG2017]
[DSG2017]	(Dutta+Srianand+Gupta+, 2017)
Write:	<<[DSG2017] JHHMMSS.ss+DDMMSS.s>>
N:	62
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	GMRT, VLA and WSRT HI 21-cm line absorption observations of N=62 radio sources.
Ref:	=2017MNRAS.465..588D
by	DUTTA R. , SRIANAND R., GUPTA N., MOMJIAN E., NOTERDAEME P., PETITJEAN P., RAHMANI H.
	Mon. Not. R. Astron. Soc., 465, 588-618 (2017)
	H I 21-cm absorption survey of quasar-galaxy pairs: distribution of cold gas around z < 0.4 galaxies.
o	Table Aa: <[DSG2017] JHHMMSS.ss+DDMMSS.s> N=62.
=E=	Catalogue in electronic form as <J/MNRAS/465/588/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSG97]
[DSG97]	(Dalcanton+Spergel+Gunn+, 11997)
Write:	<<[DSG97] A-NNN-N>>
N:	7
Object:	G (SIMBAD class: LowSurfBrghtG = Low Surface Brightness Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=7 low-surface brightness galaxies from a large survey, in the format the letter 'A' stands for 4 substrips 'M, N , Q, R' The authors used existing imaging data, originally taken for the Palomar Transit Grism Survey.
Ref:	=1997AJ....114..635D
by	DALCANTON J.J. , SPERGEL D.N., GUNN J.E., SCHMIDT M., SCHNEIDER D.P.
	Astron. J., 114, 635-654 (1997)
	The number density of low-surface brightness galaxies with 23<µ.0<25 V mag/arcsec2.
o	(Erratum) Erratum 1997, AJ vol. 114, p. 2178
o	Table 1: <[DSG97] A-NNN-N> N=7
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DSH
DSH	(Deep Sky Hunters Catalogue)
Write:	<<DSH JHHMM.m+DDMMA>>
N:	about 800
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	We present a list of previously unknown deep-sky candidate objects (open clusters, diffuse nebulae, planetary nebulae, and galaxies), which were found through visual inspection of DSS and 2MASS images and, in the case of open star clusters, via proper motion analyses using various astrometric catalogues. The possible existence of these stellar agglomerations is supported by the analysis of proper motions, color-magnitude diagrams, stellar density distributions, and by their visual appearance on DSS and 2MASS images. We provide positions, sizes of the cluster candidates, as well as preliminary results of the analysis. The DSH collaboration (http://groups.yahoo.com/group/deepskyhunters) is a group of amateur and professional astronomers founded in June 2003. Its intentions are the discovery of deep sky objects not yet published in professional literature and the improvment of observational data for already known objects. See also Alessi. 2006A&A...447..921K: first ref. with DSH objects.
Ref:	=2006A&A...447..921K
by	KRONBERGER M. , TEUTSCH P., ALESSI B., STEINE M., FERRERO L., GRACZEWSKI K., JUCHERT M., PATCHICK D., RIDDLE D., SALORANTA J., SCHOENBALL M., WATSON C.
	Astron. Astrophys., 447, 921-928 (2006)
	New galactic open cluster candidates from DSS and 2MASS imagery.
o	Tables: <DSH JHHMM.m+DDMMA> N=90.
=E=	Catalogue in electronic form as J/A+A/447/921
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [DSH2001]
[DSH2001]	(Dufton+Smartt+Hambly, 2001)
Write:	<<[DSH2001] FFF-NN>>
N:	58+61+64+64+63+61+61
Object:	Blue * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	UKST survey of Blue stellar candidates in 7 Galactic Center fields 'FFF'. See also [DSH99].
Ref:	=2001A&A...373..608D
by	DUFTON P.L. , SMARTT S.J., HAMBLY N.C.
	Astron. Astrophys., 373, 608-624 (2001)
	A UKST survey of blue objects towards the Galactic Centre - seven additional fields.
o	Table 2: <[DSH2001] 279-NN> (Nos 1-58). Table 3: <[DSH2001] 333-NN> (Nos 1-61). Table 4: <[DSH2001] 391-NN> (Nos 1-64). Table 5: <[DSH2001] 520-NN> (Nos 1-64). Table 6: <[DSH2001] 522-NN> (Nos 1-63). Table 7: <[DSH2001] 589-NN> (Nos 1-61). Table 8: <[DSH2001] 591-NN> (Nos 1-61).
=E=	Catalogue in electronic form as J/A+A/373/608
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSH2013]
[DSH2013]	(Ducci+Sasaki+Haberl+, 2013)
Write:	<<[DSH2013] NNN>>
N:	189
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton observations of N=189 sources in M83.
in source:	M 83 = NGC 5236
Ref:	=2013A&A...553A...7D
by	DUCCI L. , SASAKI M., HABERL F., PIETSCH W.
	Astron. Astrophys., 553A, 7-7 (2013)
	X-ray source population study of the starburst galaxy M 83 with XMM-Newton.
o	Tables B.1-B.2: <[DSH2013] NNN> (Nos 1-189).
=E=	Catalogue in electronic form as J/A+A/553/A7
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSH86]
[DSH86]	(Dietz+Smith+Hackwell+, 1986)
Write:	<<[DSH86] KN>>
N:	6
Object:	Feature (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
in source:	M 82 = NGC 3034
Ref:	=1986AJ.....91..758D
by	DIETZ R.D. , SMITH J., HACKWELL J.A., GEHRZ R.D., GRASDALEN G.L.
	Astron. J., 91, 758-760 (1986)
	Morphology of the nuclear region of M 82 at 2.2 µ.
o	Table 2: <[DSH86] KN> (Nos K1-K6)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSH95]
[DSH95]	(Duncan+Stewart+Haynes+, 1995)
Write:	<<[DSH95] LLL+B>> <<[DSH95] LLL.l+B.b>>
N:	33+11
Object:	Poss. SNR (SIMBAD class: SNRemnant_Candidate = SuperNova Remnant Candidate)
Stat:	is completely incorporated in Simbad
Note:	Tables 4, 6
Ref:	=1995MNRAS.277...36D
by	DUNCAN A.R. , STEWART R.T., HAYNES R.F., JONES K.L.
	Mon. Not. R. Astron. Soc., 277, 36-52 (1995)
	A deep radio continuum survey of the southern Galactic plane at 2.4 GHz.
o	Tables 4, 6: <[DSH95] LLL+B>, <[DSH95] LLL.l+B.b>, N=33
Ref:	=1997MNRAS.287..722D
by	DUNCAN A.R. , STEWART R.T., HAYNES R.F., JONES K.L.
	Mon. Not. R. Astron. Soc., 287, 722-738 (1997)
	Supernova remnant candidates from the Parkes 2.4-GHz survey.
o	p. 736, objects GLLL.ll+B.b are IRAS in SIMBAD
o	Table 1: <[DSH95] LLL+B>, <[DSH95] LLL.l+B.b> N=11 are new
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSH99]
[DSH99]	(Dufton+Smartt+Hambly, 1999)
Write:	<<[DSH99] FFF-NN>>
N:	240
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	UKST survey towards the Galactic Center in 19 'FFF' UKST fields. 1999A&AS..139..231D: Preliminary results in 3 UKST fields. See also [DSH2001].
in source:	NAME Gal Center
Ref:	=1999A&AS..139..231D
by	DUFTON P.L. , SMARTT S.J., HAMBLY N.C.
	Astron. Astrophys., Suppl. Ser., 139, 231-244 (1999)
	A UKST survey of blue objects towards the galactic centre - a search for early-type stars.
o	Tables 2-5: <[DSH99] 393-NN> (Nos 1-80), <[DSH99] 454-NN> (Nos 1-80), <[DSH99] 456-NN> (Nos 1-80).
=E=	Catalogue in electronic form as J/A+AS/139/231
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSJ85]
[DSJ85]	(De Pater+Schloerb+Johnson, 1985)
Write:	<<[DSJ85] HHMM+DDdA>>
N:	8+101+56
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Table I: N=8 calibrator sources. Table II: N=101 sources to be occulted by Halley comet. Table III: N=56 sources to be occulted by Giacobini-Zinner comet
Ref:	=1985AJ.....90..846D
by	DE PATER I. , SCHLOERB F.P., JOHNSON A.H.
	Astron. J., 90, 846-868 (1985)
	A catalog of radio sources to be occulted by comets P/Halley and P/Giacobini-Zinner.
o	Tables I, II, III: <[DSJ85] HHMM+DDdA> N=8+101+56
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSL2000]
[DSL2000]	(Dagkesamanskii+Samodurov+Lapaev, 2000)
Write:	<<[DSL2000] HHMM+DDd>>
N:	920
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=2000ARep...44...18D
by	DAGKESAMANSKII R.D. , SAMODUROV V.A., LAPAEV K.A.
	Astron. Rep., 44, 18-25 (2000)
	A sky survey at 102.5 MHz: radio sources at declinations 27.5 °-33.5 ° and 67.5 °-70.5 °.
o	=2000AZh....77...21D
o	Tables 2, 3: <[DSL2000] HHMM+DDd> N=920.
=E=	Catalogue in electronic form as J/AZh/77/21
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSL2008]
[DSL2008]	(Davis+Scholz+Lucas+, 2008)
Write:	<<[DSL2008] NN>>
N:	85
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	UKIRT WFCAM narrow-band H2 observations of the Taurus-Auriga-Perseus region.
in source:	NAME Tau Aur Per Complex
Ref:	=2008MNRAS.387..954D
by	DAVIS C.J. , SCHOLZ P., LUCAS P., SMITH M.D., ADAMSON A.
	Mon. Not. R. Astron. Soc., 387, 954-968 (2008)
	A shallow though extensive H_{2}2.122-µm imaging survey of Taurus-Auriga-Perseus - I. NGC 1333, L1455, L1448 and B1.
o	Table A1: <[DSL2008] NN> (Nos 1-85).
=E=	Catalogue in electronic form as J/MNRAS/387/954
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSM2002]
[DSM2002]	(Donahue+Scharf+Mack+, 2002)
Write:	<<[DSM2002] OCNNa JHHMM+DDMM>>
N:	155
Object:	Poss. Cluster of G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Comparison of optical and ROSAT X-ray catalogs of candidate clusters of galaxies (letters OC in the format stands for Optical Candidate.)
Ref:	=2002ApJ...569..689D
by	DONAHUE M. , SCHARF C.A., MACK J., LEE Y.P., POSTMAN M., ROSATI P., DICKINSON M., VOIT G.M., STOCKE J.T.
	Astrophys. J., 569, 689-719 (2002)
	Distant cluster hunting. II. A comparison of X-ray and optical cluster detection techniques and catalogs from the ROSAT optical X-ray survey.
o	Table 2: <[DSM2002] OCNNa JHHMM+DDMM> N=155.
=E=	Catalogue in electronic form as J/ApJ/569/689
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSM2005]
[DSM2005]	(Doroshenko+Sergeev+Merkulova+, 2005)
Write:	<<[DSM2005] W Com N>> <<[DSM2005] NGC NNNN N>> <<[DSM2005] 3C NNN N>> <<[DSM2005] 3C 390.3 NN>> <<[DSM2005] Mrk NNN N>> <<[DSM2005] PKS 1510-089 N>> <<[DSM2005] PG 1553+11 N>> <<[DSM2005] Arp 102B N>> <<[DSM2005] 1E 1821+64.3 N>> <<[DSM2005] OX 169 N>> <<[DSM2005] BL Lac NN>> <<[DSM2005] Akn 564 NN>>
N:	126
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	CDD BVRI observations of comparison stars in the field of Seyfert galaxies, with the 70 cm telescope of the Crimean Astrophysical Observatory.
Ref:	=2005Ap.....48..304D
by	DOROSHENKO V.T. , SERGEEV S.G., MERKULOVA N.I., SERGEEVA E.A., GOLUBINSKY Y.V., PRONIK V.I., OKHMAT N.N.
	Astrophysics, 48, 304-320 (2005)
	BVRI CCD-Photometry of comparison stars in the neighborhood of galaxies with active nuclei. II.
o	3C 390.3 is not identified.
o	Table 1: <[DSM2005] W Com N> (Nos 1-5), <[DSM2005] NGC NNNN N> N=4+5+6+9+5, <[DSM2005] 3C NNN.N N> N=4+6+9, <[DSM2005] Mrk NNN N> N=5+5, <[DSM2005] PKS 1510-089 N> (Nos 1-7), <[DSM2005] PG 1553+11 N> (Nos 1-8, 6 missing), <[DSM2005] Arp 102B N> (Nos 1-6), <[DSM2005] 1E 1821+64.3 N> (Nos 1-8), <[DSM2005] OX 169 N> N=7 among (Nos 1-9), <[DSM2005] BL Lac NN> N=10 among (Nos 3-31). <[DSM2005] Akn 564 NN> (Nos 0-13, 4, 6 missing).
=E=	Catalogue in electronic form as J/other/Ap/48.304
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSM2016]
[DSM2016]	(Deneva+Stovall+Mclaughlin+, 2016)= (RRAT)
Write:	<<[DSM2016] JHHMM+DD>>
N:	8
Object:	Psr (SIMBAD class: Pulsar)
Stat:	is completely incorporated in Simbad
Note:	N=8 Rotating Radio Transients (RRATs) discovered with the Clusterrank algorithm. Use of Arecibo 327MHz Drift Pulsar Survey. A list of the properties of Rotating Radio Transients in different surveys can be found here: http://astro.phys.wvu.edu/rratalog/.br See also [MLL2006], [MLL2006] and [KKL2015].
Ref:	=2016ApJ...821...10D
by	DENEVA J.S. , STOVALL K., McLAUGHLIN M.A., BAGCHI M., BATES S.D., FREIRE P.C.C., MARTINEZ J.G., JENET F., GARVER-DANIELS N.
	Astrophys. J., 821, 10-10 (2016)
	New discoveries from the Arecibo 327 MHz drift pulsar survey radio transient search.
o	Table 4: <[DSM2016] JHHMM+DD> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSM2019]
[DSM2019]	(Dobie+Stewart+Murphy+, 2019)= (ASKAP) (Not yet in Simbad)
Write:	<<[DSM2019] ASKAP JHHMMSS.s+DDMMSS>>
N:	21
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Australian Square Kilometer Array Pathfinder (ASKAP) observations of N=21 candidate counterparts in search for a radio transient associated with the LIGO/Virgo source S190814bv.
Ref:	=2019ApJ...887L..13D
by	DOBIE D. , STEWART A., MURPHY T., LENC E., WANG Z., KAPLAN D.L., ANDREONI I., BANFIELD J., BROWN I., CORSI A., DE K., GOLDSTEIN D.A., HALLINAN G., HOTAN A., HOTOKEZAKA K., JAODAND A.D., KARAMBELKAR V., KASLIWAL M.M., McCONNELL D., MOOLEY K., MOSS V.A., NEWMAN J.A., PERLEY D.A., PRAKASH A., PRITCHARD J., SADLER E.M., SHARMA Y., WARD C., WHITING M., ZHOU R.
	Astrophys. J., 887L, 13-13 (2019)
	An ASKAP search for a radio counterpart to the first high-significance neutron star-black hole merger LIGO/Virgo S190814bv.
o	Table 2: <[DSM2019] ASKAP JHHMMSS.s+DDMMSS> N=21.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSM2020]
[DSM2020]	(Darvish+Scoville+Martin+, 2020)
Write:	<<[DSM2020] COSMOS Cluster 2.2>> <<[DSM2020] CC2.2>> (not recognised by Simbad, but found in literature)
N:	1
Object:	Protocluster (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Keck I MOSFIRE osbervations of N=1 protocluster at z∼2.2 in the COSMOS field.
in source:	NAME COSMOS Field
Ref:	=2020ApJ...892....8D
by	DARVISH B. , SCOVILLE N.Z., MARTIN C., SOBRAL D., MOBASHER B., RETTURA A., MATTHEE J., CAPAK P., CHARTAB N., HEMMATI S., MASTERS D., NAYYERI H., O'SULLIVAN D., PAULINO-AFONSO A., SATTARI Z., SHAHIDI A., SALVATO M., LEMAUX B.C., LE FEVRE O., CUCCIATI O.
	Astrophys. J., 892, 8-8 (2020)
	Spectroscopic confirmation of a Coma Cluster progenitor at z ~ 2.2.
o	Fig. 1, Table 2: <[DSM2020] COSMOS Cluster 2.2> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSM97]
[DSM97]	(Deguchi+Shiki+Matsumoyo+, 1997) (Not yet in Simbad)
Write:	<<[DSM97] A>>
N:	5
Object:	Source (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 2: (Nos A-C) SiO sources in the field of [SOD97] 5, (Nos D-E) SiO sources in the field of [SOD97] 6. Maps figs 2b 2c
in source:	[SOD97] 5
in source:	[SOD97] 6
Ref:	=1997PASJ...49..561D
by	DEGUCHI S. , SHIKI S., MATSUMOTO S., JIANG B., NAKADA Y., WOOD P.
	Publ. Astron. Soc. Jap., 49, 561-569 (1997)
	Infrared identification of SiO maser sources toward the Sgr B2 molecular cloud.
o	Sgr B2 MD5 = [MD72] 5
o	Table 2: <[DSM97] A> (Nos A-E)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSM98]
[DSM98]	(Davis+Smith+Moriarty-Schieven, 1998)
Write:	<<[DSM98] W75N A>> <<[DSM98] W75N WW>>
N:	8+2
Object:	Knot + Region (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Fig.1, Table 1: N=7 H2 Knots in W 75N, (Nos A-H), Map. N=2 regions in W 75N, (Nos NE and SW) See also [STS2003].
in source:	W 75:W 75N = W 75N
Ref:	=1998MNRAS.299..825D
by	DAVIS C.J. , SMITH M.D., MORIARTY-SCHIEVEN G.H.
	Mon. Not. R. Astron. Soc., 299, 825-833 (1998)
	A textbook case of bow shock entrainment in a YSO outflow.
o	Fig.1, Table 1: <[DSM98] W75N A> (Nos A-H), <[DSM98] W75N WW> (Nos NE, SW).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSO2004]
[DSO2004]	(Dolphin+Saha+Olszewski+, 2004)
Write:	<<[DSO2004] VNN>>
N:	37
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	WIYN telescope observations. New search for RR Lyrae in an M 31 halo field located 40' from the nucleus of the galaxy along the minor axis. Finding chart in Fig.8. See also PvdB.
in source:	M 31 = NGC 224
Ref:	=2004AJ....127..875D
by	DOLPHIN A.E. , SAHA A., OLSZEWSKI E.W., THIM F., SKILLMAN E.D., GALLAGHER J.S., HOESSEL J.
	Astron. J., 127, 875-896 (2004)
	Short-period variable stars in the M31 halo.
o	Table 2: <[DSO2004] VNN> (Nos V01-V37).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSO2007]
[DSO2007]	(Donahue+Sun+O'Dea+, 2007)
Write:	<<[DSO2007] A>> <<[DSO2007] WW filament>>
N:	2+2
Object:	G in ClG + Part of G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	SOAR telescope observations of the cluster 2A 0335+096. A and B are respectively the brightest cluster galaxy and its companions. N=2 H-alpha filaments are alos observed.
in source:	2A 0335+096
Ref:	=2007AJ....134...14D
by	DONAHUE M. , SUN M., O'DEA C.P., VOIT G.M., CAVAGNOLO K.W.
	Astron. J., 134, 14-25 (2007)
	Star formation, radio sources, cooling X-ray gas, and galaxy interactions in the brightest cluster galaxy in 2A0335+096.
o	brightest cluster galaxy in 2A0335+096 is [SBO95] 1.
o	Table 1: <[DSO2007] A> (Nos A-B), <[DSO2007] WW filament> (Nos NW, SE).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSO99]
[DSO99]	(Da Costa+Scodeggio+Olsen+, 1999)= (EIS)
Write:	<<[DSO99] EIS JHHMM+DDMM>> <<[DSO99] EIS JHHMM+DDMM NN>>
N:	2+10+10
Object:	Cluster of G + G in ClG (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 2: N=2 EIS (ESO Imaging Survey) clusters. Fig.2: N=10 brightest galaxies in the 2 clusters. See also [SOD99], [OSD99].
Ref:	=1999A&A...343L..29D
by	DA COSTA L. , SCODEGGIO M., OLSEN L.F., NONINO M., RENGELINK R., BENDER R., FRANX M., JORGENSEN H.E., RENZINI A., ROSATI P.
	Astron. Astrophys., 343, 29-34 (1999)
	VLT and NTT observations of two EIS cluster candidates. Detection of the early-type galaxies sequence at z~1.
o	Table 2: <[DSO99] EIS JHHMM+DDMM> N=2. Fig.2: <[DSO99] J0046-2930 NN> N=10, <[DSO99] J0046-2951 NN> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSP2007]
[DSP2007]	(Dahm+Simon+Proszkow+, 2007)= (UHX)
Write:	<<[DSP2007] NNN>>
N:	300
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton EPIC observations of NGC 2264.
in source:	NGC 2264
Ref:	=2007AJ....134..999D
by	DAHM S.E. , SIMON T., PROSZKOW E.M., PATTEN B.M.
	Astron. J., 134, 999-1018 (2007)
	X-ray observations of the young cluster NGC 2264.
o	Table 2: <[DSP2007] NNN> (Nos 1-300).
=E=	Catalogue in electronic form as J/AJ/134/999
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSP2017]
[DSP2017]	(Davidge+Serjeant+Pearson+, 2017)
Write:	<<[DSP2017] JDDD.dddd+DD.dddd>>
N:	905+625+2885
Object:	G (SIMBAD class: Galaxy)
Note:	Catalogues of N=905+625+2885 galaxies in three extragalactic fields (IRAC Dark Field, ELAIS N1, ADF-S), based on AKARI IRC images.
in source:	ELAIS N1
Ref:	=2017MNRAS.472.4259D
by	DAVIDGE H. , SERJEANT S., PEARSON C., MATSUHARA H., WADA T., DRYER B., BARRUFET L.
	Mon. Not. R. Astron. Soc., 472, 4259-4286 (2017)
	AKARI/IRC source catalogues and source counts for the IRAC Dark Field, ELAIS North and the AKARI Deep Field South.
o	<[DSP2017] JDDD.dddd+DD.dddd> N=905+625+2885.
=E=	Catalogue in electronic form as J/MNRAS/472/4259
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSP99]
[DSP99]	(Dressler+Smail+Poggianti+, 1999)
Write:	<<[DSP99] A370 NN>> <<[DSP99] Cl HHMM+DD NNN>> <<[DSP99] 3C 295 NN>>
N:	424+253
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of galaxies in 10 ClG. Table 4a: N=424 galaxies in ClG. Table 4b: N=253 galaxies in ClG field.
in source:	ACO 370
in source:	ClG 1447+26
in source:	ClG 0024+1652 = HMS 0024+1654
in source:	ClG 0939+4713 = ACO 851
in source:	ClG 0303+1706
in source:	ClG 0412-6559
in source:	ClG 1601+4253
in source:	ClG 0016+1609 = 1E 0015.9+1609
in source:	ClG 0054-27
in source:	NAME 3C 295 Cluster
Ref:	=1999ApJS..122...51D
by	DRESSLER A. , SMAIL I., POGGIANTI B.M., BUTCHER H., COUCH W.J., ELLIS R.S., OEMLER A.Jr
	Astrophys. J., Suppl. Ser., 122, 51-80 (1999)
	A spectroscopic catalog of 10 distant rich clusters of galaxies.
o	The printed version gives a truncated format Cl HHMM. The complete format is ClG HHMM+DD in Simbad.
o	Tables 4a, 4b: <[DSP99] A 370 NNN>, <[DSP99] Cl HHMM+DD NNN>, <[DSP99] 3C 295 NNN>, N=424+253.
=E=	Catalogue in electronic form as J/ApJS/122/51
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSR2005]
[DSR2005]	(Dirsch+Schuberth+Richtler, 2005)
Write:	<<[DSR2005] JHHMMSS.ss+DDMMSS.s>>
N:	16277
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	CTIO 4m Blanco telescope MOSAIC observations of NGC 4636.
in source:	NGC 4636
Ref:	=2005A&A...433...43D
by	DIRSCH B. , SCHUBERTH Y., RICHTLER T.
	Astron. Astrophys., 433, 43-56 (2005)
	A wide-field photometric study of the globular cluster system of NGC 4636.
o	Table a1: <[DSR2005] JHHMMSS.ss+DDMMSS.s> N=16277.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSR2006]
[DSR2006]	(Danforth+Shull+Rosenberg+, 2006) (Not yet in Simbad)
Write:	<<[DSR2006] QSO JHHMM+DDMM abs N.NNNNN>>
N:	171
Object:	Absorber
Note:	171 strong Ly-alpha absorption lines in 31 AGNs.
Ref:	=2006ApJ...640..716D
by	DANFORTH C.W. , SHULL J.M., ROSENBERG J.L., STOCKE J.T.
	Astrophys. J., 640, 716-740 (2006)
	The low-z intergalactic medium. II. Lyβ, O VI, and C III forest.
o	LBQS 1343+264 A/B = QSO B1343+2640A, QSO B1343+2640B
o	Table 2: <[DSR2006] QSO JHHMM+DDMM abs N.NNNNN> N=171.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSR2012]
[DSR2012]	(Das+Sengupta+Ramya+, 2012) (Not yet in Simbad)
Write:	<<[DSR2012] NGC NNNN N>>
N:	4+8
Object:	H-alpha emission region (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Himalayan Chandra 2m telescope (HCT, India) observations of N=4+8 Hα emission regions in NGC 3445 and NGC 4027 respectively.
in source:	NGC 3445
in source:	NGC 4027
Ref:	=2012MNRAS.423.3274D
by	DAS M. , SENGUPTA C., RAMYA S., MISRA K.
	Mon. Not. R. Astron. Soc., 423, 3274-3284 (2012)
	Star formation in bulgeless late-type galaxies: clues to their evolution.
o	Figs 6-7, Table 3: <[DSR2012] NGC 3445 N> (Nos 1-4), <[DSR2012] NGC 4027 N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSR86]
[DSR86]	(Dressler+Schechter+Rose, 1986)
Write:	<<[DSR86] NGC 720 NN>>
N:	7
Object:	G (SIMBAD class: Galaxy)
Note:	N=6 faint companions and one unconfirmed seventh among the 14 galaxies in the field around NGC 720.
Ref:	=1986AJ.....91.1058D
by	DRESSLER A. , SCHECHTER P.L., ROSE J.A.
	Astron. J., 91, 1058-1061 (1986)
	The mass of the isolated elliptical NGC 720 as determined from the dynamics of its companions.
o	Table 1: <[DSR86] NGC 720 NN> N=7 among (Nos 3-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DSS
DSS	(Deep Source Survey)
*****	Avoid the usage of DSS, prefer [FKW84]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [DSS2001]
[DSS2001]	(Dolphin+Saha+Skillman+, 2001)
Write:	<<[DSS2001] VNN>>
N:	24
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	HST WFPC2 photometry of IC 1613. Table 1: RR Lyrae. Table 2: Cepheid
in source:	IC 1613
Ref:	=2001ApJ...550..554D
by	DOLPHIN A.E. , SAHA A., SKILLMAN E.D., TOLSTOY E., COLE A.A., DOHM-PALMER R.C., GALLAGHER J.S., MATEO M., HOESSEL J.G.
	Astrophys. J., 550, 554-569 (2001)
	Deep Hubble space telescope imaging of IC 1613. I. Variable stars and distance.
o	Tables 1, 2: <[DSS2001] VNN> (Nos V1-V26, V11 and V12 missing).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSS2002]
[DSS2002]	(Donahue+Smith+Stocke, 2002)= ([DSS2002a])
Write:	<<[DSS2002] knot N>> <<[DSS2002] WW Arc>>
N:	6+1
Object:	Knot + Arc (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
in source:	NGC 4410A
Ref:	=2002AJ....123.1922D
by	DONAHUE M. , SMITH B.J., STOCKE J.T.
	Astron. J., 123, 1922-1936 (2002)
	Star formation in the radio galaxy NGC 4410A.
o	Fig.1, Table 2: <[DSS2002] knot N> (Nos 1-6), <[DSS2002] NW Arc> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSS2002a]
[DSS2002a]	(Donahue+Smith+Stocke, 2002)
*****	Avoid the usage of [DSS2002a], prefer [DSS2002]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSS2002b]
[DSS2002b]	(Dawson+Spinrad+Stern+, 2002)
Write:	<<[DSS2002b] ES1>> <<[DSS2002b] D16>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck telescope observations.
Ref:	=2002ApJ...570...92D
by	DAWSON S. , SPINRAD H., STERN D., DEY A., VAN BREUGEL W., DE VRIES W., REULAND M.
	Astrophys. J., 570, 92-99 (2002)
	A galactic wind at z=5.190.
o	Fig.7: galaxy RD 581 (z=4.89) not identified.
o	Fig.2: <[DSS2002b] ES1> N=1, <[DSS2002b] D16> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSS2003]
[DSS2003]	(Dolphin+Saha+Skillman+, 2003)
Write:	<<[DSS2003] CN-VNN>>
N:	13+19+24+26
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Note:	HST WFPC2 observations of Sextans B. Identification of 82 short-period variable stars. In the format 'CN' stands for Chips C1, C2, C3, C4. See also 2002AJ....123..813D (Paper I).
in source:	Sextans A = DDO 75
Ref:	=2003AJ....125.1261D
by	DOLPHIN A.E. , SAHA A., SKILLMAN E.D., DOHM-PALMER R.C., TOLSTOY E., COLE A.A., GALLAGHER J.S., HOESSEL J.G., MATEO M.
	Astron. J., 125, 1261-1290 (2003)
	Deep Hubble Space Telescope imaging of Sextans A. II. Cepheids and distance.
o	Table 2: <[DSS2003] CN-VNN> N-13+19+24+26.
=E=	Catalogue in electronic form as J/AJ/125/1261
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSS2007]
[DSS2007]	(Dye+Smail+Swinbank+, 2007) (Not yet in Simbad)
Write:	<<[DSS2007] A>>
N:	3
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	HST ACS observations of the field of the LBG [SSR2007] LBG J213512.73-010143. N=3 galaxies likely members of the cluster MCS J2135.2-0102.
in source:	MCS J2135.2-0102 = ClG J2135-0102
Ref:	=2007MNRAS.379..308D
by	DYE S. , SMAIL I., SWINBANK A.M., EBELING H., EDGE A.C.
	Mon. Not. R. Astron. Soc., 379, 308-316 (2007)
	Separation of the visible and dark matter in the Einstein ring LBG J213512.73-010143.
o	Fig.1: <[DSS2007] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSS2008]
[DSS2008]	(De Mello+Smith+Sabri+, 2008)
Write:	<<[DSS2008] N>>
N:	8
Object:	(Far UV) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	GALEX UV observations of N=8 young star-forming regions in the HI Bridge between M 81 and M 82 ([ADS81] 1).
in source:	[ADS81] I
Ref:	=2008AJ....135..548D
by	DE MELLO D.F. , SMITH L.J., SABBI E., GALLAGHER J.S., MOUNTAIN M., HARBECK D.R.
	Astron. J., 135, 548-554 (2008)
	Star formation in the H I bridge between M81 and M82.
o	Fig.5, Table 1: <[DSS2008] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSS2017]
[DSS2017]	(Danielson+Swinbank+Smail+, 2017)
Write:	<<[DSS2017] NNNNNNNNa>>
N:	1708
Object:	G (SIMBAD class: Galaxy)
Note:	VLT (FORS2, VIMOS and XSHOOTER), Keck I (MOSFIRE), Keck II (DEIMOS), and Gemini (GNIRS) observations of N=1708 galaxies in the extended Chandra Deep Field South.
in source:	NAME ECDFS
Ref:	=2017ApJ...840...78D
by	DANIELSON A.L.R. , SWINBANK A.M., SMAIL I., SIMPSON J.M., CASEY C.M., CHAPMAN S.C., DA CUNHA E., HODGE J.A., WALTER F., WARDLOW J.L., ALEXANDER D.M., BRANDT W.N., DE BREUCK C., COPPIN K.E.K., DANNERBAUER H., DICKINSON M., EDGE A.C., GAWISER E., IVISON R.J., KARIM A., KOVACS A., LUTZ D., MENTEN K., SCHINNERER E., WEISS A., VAN DER WERF P.
	Astrophys. J., 840, 78-78 (2017)
	An ALMA survey of submillimeter galaxies in the Extended Chandra Deep Field South: spectroscopic redshifts.
o	Table 1: <[DSS2017] NNNNNNNNa> N=1708 among (Nos 101-99944000).
=E=	Catalogue in electronic form as <J/ApJ/840/78/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSS2020]
[DSS2020]	(Della Costa+Sarajedini+Strolger, 2020)
Write:	<<[DSS2020] MACSJ1149 NN>> <<[DSS2020] SN Dellanova>> <<[DSS2020] SN Saranova>> <<[DSS2020] MACSJ1149 CN>>
N:	49+1+1+2
Object:	Poss. AGN + SN + Poss. SN (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=49 AGN candidates, N=2 SN, and N=2 SN candidates in the field of MCS J1149.5+2223. Use of HST archival images of MCS J1149.5+2223.
in source:	ClG J1149+2223 = MCS J1149.5+2223
Ref:	=2020ApJ...894...56D
by	DELLA COSTA J. , SARAJEDINI V.L., STROLGER L.-G.
	Astrophys. J., 894, 56-56 (2020)
	Decadal variability survey in MACSJ1149.
o	Table 2: <[DSS2020] MACSJ1149 NN> (Nos 1-49). Table 3: <[DSS2020] SN Dellanova> N=1, <[DSS2020] SN Saranova> N=1, <[DSS2020] MACSJ1149 CN> (Nos C1-C2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSS98]
[DSS98]	(Dey+Spinrad+Stern+, 1998)
Write:	<<[DSS98] 0140+326 BDNN>> <<[DSS98] 0140+326 RDN>> <<[DSS98] Star A>>
N:	3+1
Object:	G + * (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	In the format 'RD' stands for 'Red Dropout' and 'BD' for 'Blue Dropout'. N=3 galaxies + N=1 star in the field of 6C 0140+3238.
Ref:	=1998ApJ...498L..93D
by	DEY A. , SPINRAD H., STERN D., GRAHAM J.R., CHAFFEE F.H.
	Astrophys. J., 498, 93-98 (1998)
	A galaxy at z=5.34.
o	Table 1, Fig.1: <[DSS98] 0140+326 BD3>, <[DSS98] 0140+326 RD1>, <[DSS98] Star A>
Ref:	=1999PASP..111.1475S
by	STERN D. , SPINRAD H.
	Publ. Astron. Soc. Pac., 111, 1475-1502 (1999)
	Search techniques for distant galaxies. (Invited review).
o	p.1489: PKS 1614-051 misprint for +051. Fig.8: [MSS2000] SSA 22 ser N (Nos 1-2).
o	Fig.4: <[DSS98] 0140+326 BDNN> (No. BD12) added. Fig.8: <[SGP96] SSA 22 ANN> (No. C17) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DSW
DSW	(Debes+Sigurdsson+Woodgate)
Write:	<<DSW N>> <<DSW WD HHMM+DDd CN>>
N:	4+13
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST survey of nearby WD*. 4 extragalactic objects are found. Possible companions of 4 white dwarfs are studied.
Ref:	=2005AJ....130.1221D
by	DEBES J.H. , SIGURDSSON S., WOODGATE B.E.
	Astron. J., 130, 1221-1230 (2005)
	Cool customers in the stellar graveyard. II. Limits to substellar objects around nearby DAZ white dwarfs.
o	Table 3: <DSW N> (Nos 1-4). Figs 1-4: <DSW 2326+049 CN> (No. C1), <DSW 0208+395 CN> (Nos C1-C2), <DSW 0245+541 CN> (Nos C1-C3), <DSW 1620-391 CN> (Nos C1-C7).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DSW2017]
[DSW2017]	(Dong+Schodel+Williams+, 2017)
Write:	<<[DSW2017] NNNNN>>
N:	33070
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	HST WFC3 IR observations of N=33070 variable stars in the Milky Way nuclear star cluster.
in source:	NAME Galactic Center Cluster
Ref:	=2017MNRAS.470.3427D
by	DONG H. , SCHODEL R., WILLIAMS B.F., NOGUERAS-LARA F., GALLEGO-CANO E., GALLEGO-CALVENTE T., WANG Q.D., MORRIS M.R., DO T., GHEZ A.
	Mon. Not. R. Astron. Soc., 470, 3427-3452 (2017)
	Near-infrared variability study of the central 2.3 arcmin x 2.3 arcmin of the Galactic Centre - I. Catalogue of variable sources.
o	<[DSW2017] NNNNN> (Nos 1-33070).
=E=	Catalogue in electronic form as J/MNRAS/470/3427
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DSW98]
[DSW98]	(Davies+Sugai+Ward, 1998) (Not yet in Simbad)
Write:	<<[DSW98] A>>
N:	15
Object:	Region (SIMBAD class: Region = Region defined in the Sky)
in source:	NGC 1068
Ref:	=1998MNRAS.300..388D
by	DAVIES R.I. , SUGAI H., WARD M.J.
	Mon. Not. R. Astron. Soc., 300, 388-396 (1998)
	Star formation in the circumnuclear environment of NGC 1068.
o	Fig1, Tables 1, 2: <[DSW98] A> (Nos A-O).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DT2000]
[DT2000]	(Dahlem+Thiering, 2000)
Write:	<<[DT2000] NGC 4104 NN>> <<[DT2000] NGC 6269 NN>> <<[DT2000] NGC 6329 NN>>
N:	27+17+39
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations of 3 poor clusters of galaxies. Table 7: N=27 sources in the field of NGC 4104. Table 8: N=17 sources in the field of NGC 6269. Table 9: N=39 sources in the field of NGC 6329.
in source:	MKW 4s
in source:	AWM 5
in source:	NAME NGC 6329 GROUP
Ref:	=2000PASP..112..148D
by	DAHLEM M. , THIERING I.
	Publ. Astron. Soc. Pac., 112, 148-162 (2000)
	Diffuse X-ray emission in three poor clusters of galaxies.
o	Table 7: <[DT2000] NGC 4104 NN> (Nos 1-27). Table 8: <[DT2000] NGC 6269 NN> (Nos 1-17). Table 9: <[DT2000] NGC 6329 NN> (Nos 1-39).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DT85]
[DT85]	(Dame+Thaddeus, 1985)
Write:	<<[DT85] Cloud A>>
N:	3
Object:	Cloud (SIMBAD class: Cloud)
Note:	N=3 clouds in the Great Rift system.
in source:	NAME Great Rift
Ref:	=1985ApJ...297..751D
by	DAME T.M. , THADDEUS P.
	Astrophys. J., 297, 751-765 (1985)
	A wide-latitude CO survey of molecular clouds in the Northern Milky Way.
o	Table 4: <[DT85] Cloud A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DTARPS-E
DTARPS-E	(DIAmante TESS AutoRegressive Planet Search Ecliptic) (Not yet in Simbad)
Write:	<<DTARPS-E NNN>>
Object:	Stars (SIMBAD class: Star)
Note:	A future catalog based on the TESS survey of the ecliptic pole regions, using the AutoRegressive Planet Search (ARPS) methodology, a novel sequence of statistical procedures for detecting transiting planetary candidates from photometric surveys. See DTARPS-S for more information.
Auth.:	Eric Feigelson Penn State University
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: DTARPS-N
DTARPS-N	(DIAmante TESS AutoRegressive Planet Search North) (Not yet in Simbad)
Write:	<<DTARPS-N NNN>>
Object:	Stars (SIMBAD class: Star)
Note:	The AutoRegressive Planet Search (ARPS) methodology is a novel sequence of statistical procedures for detecting transiting planetary candidates from photometric surveys. It complements official candidate lists such as the Kepler Objects of Interest and TESS Objects of Interest. The methodology is described by Caceres, Feigelson et al. (2019AJ....158...58C) and Melton, Feigelson et al. (2024AJ....167..202M). The ARPS methodology produces catalogs that are both sensitive to smaller planets and relatively free of contaminating False Positive and False Alarm. The procedure has been applied to the 4-year Kepler survey (Caceres, Feigelson et al. 2019AJ....158...58C), and has been applied to the TESS Year 1 survey of the southern sky (DTARPS-S). A similar catalog is being prepared based on the TESS Year 2 survey of the northern hemisphere. See also DTARPS-E for a future catalog based on the TESS survey of the ecliptic pole regions.
Auth.:	Eric Feigelson Penn State University
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: DTARPS-S
DTARPS-S	(DIAmante TESS AutoRegressive Planet Search South) (Not yet in Simbad)
Write:	<<DTARPS-S NNN>>
N:	462
Object:	Stars (SIMBAD class: Star)
Note:	The AutoRegressive Planet Search (ARPS) methodology is a novel sequence of statistical procedures for detecting transiting planetary candidates from photometric surveys. It complements official candidate lists such as the Kepler Objects of Interest and TESS Objects of Interest. The methodology is described by Caceres, Feigelson et al. (2019AJ....158...58C) and Melton, Feigelson et al. (2024AJ....167..202M). The ARPS methodology produces catalogs that are both sensitive to smaller planets and relatively free of contaminating False Positive and False Alarm. The procedure has been applied to the 4-year Kepler survey (Caceres, Feigelson et al. 2019AJ....158...58C), and has now been applied to the TESS Year 1 survey of the southern sky (DTARPS-S, Melton, Feigelson et al. 2024AJ....167..203M). The DTARPS-S objects are the host stars of candidate transiting planets; they generally have bright magnitudes with V<12 and are thus already in historical stellar catalogs (BD, TYC, Gaia, etc). The DTARPS-S catalog is provided in the Machine Readable Table from the Astronomical Journal (Melton, Feigelson et al. 2024AJ....167..203M).
Notes:	We are currently preparing a similar catalog based on the TESS Year 2 survey of the northern hemisphere, see DTARPS-N. In the future, we hope to produce other catalogs such as DTARPS-E from TESS survey of the ecliptic pole regions.
Ref:	=2024AJ....167..203M
Auth.:	Eric Feigelson Penn State University
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [DTB2018]
[DTB2018]	(de Ugarte Postigo+Thone+Bolmer+, 2018)
Write:	<<[DTB2018] SN>>
N:	4
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 7 (350GHz) observations of N=4 sources in the field of GRB 161023A.
Ref:	=2018A&A...620A.119D
by	DE UGARTE POSTIGO A. , THONE C.C., BOLMER J., SCHULZE S., MARTIN S., KANN D.A., D'ELIA V., SELSING J., MARTIN-CARRILLO A., PERLEY D.A., KIM S., IZZO L., SANCHEZ-RAMIREZ R., GUIDORZI C., KLOTZ A., WIERSEMA K., BAUER F.E., BENSCH K., CAMPANA S., CANO Z., COVINO S., COWARD D., DE CIA A., DE GREGORIO-MONSALVO I., DE PASQUALE M., FYNBO J.P.U., GREINER J., GOMBOC A., HANLON L., HANSEN M., HARTMANN D.H., HEINTZ K.E., JAKOBSSON P., KOBAYASHI S., MALESANI D.B., MARTONE R., MEINTJES P.J., MICHALOWSKI M.J., MUNDELL C.G., MURPHY D., OATES S., SALMON L., VAN SOELEN B., TANVIR N.R., TURPIN D., XU D., ZAFAR T.
	Astron. Astrophys., 620A, 119-119 (2018)
	X-shooter and ALMA spectroscopy of GRB 161023A. A study of metals and molecules in the line of sight towards a luminous GRB.
o	Fig. 3, Table 2: <[DTB2018] SN> (Nos S1-S4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DTD2006]
[DTD2006]	(Dasyra+Tacconi+Davies+, 2006)
Write:	<<[DTD2006] IRAS HHMMm+DDMM W>> <<[DTD2006] IRAS HHMMm+DDMM WW>>
N:	20x2
Object:	G in Pair (SIMBAD class: GinPair = Galaxy in Pair of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	VLT-ISAAC observations of ULIRGs with double nuclei.
Ref:	=2006ApJ...638..745D
by	DASYRA K.M. , TACCONI L.J., DAVIES R.I., GENZEL R., LUTZ D., NAAB T., BURKERT A., VEILLEUX S., SANDERS D.B.
	Astrophys. J., 638, 745-758 (2006)
	Dynamical properties of ultraluminous infrared galaxies. I. Mass ratio conditions for ULIRG activity in interacting pairs.
o	Table 2: <[DTD2006] IRAS HHMMm+DDMM W>, <[DTD2006] IRAS HHMMm+DDMM WW>, N=40.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DTD2010]
[DTD2010]	(Doherty+Tanaka+De Breuck+, 2010)
Write:	<<[DTD2010] MRC 0943-242 NNN>> <<[DTD2010] MRC 0943-242 HzRG>> <<[DTD2010] MRC 0943-242 LAENNNN>> <<[DTD2010] MRC 1138-262 NNN>> <<[DTD2010] JHHMMSS.ss+DDMMSS.s>>
N:	57+33
Object:	G + Radio G (SIMBAD class: Galaxy)
Note:	Subaru FOCAS and MOIRCS and VLT FORS2 observations of red galaxies in two high-redshift proto-clusters.
in source:	NAME MRC 0943-242 Protocluster
in source:	NAME Spiderweb protocluster = NAME MRC 1138-262 Protocluster
Ref:	=2010A&A...509A..83D
by	DOHERTY M. , TANAKA M., DE BREUCK C., LY C., KODAMA T., KURK J., SEYMOUR N., VERNET J., STERN D., VENEMANS B., KAJISAWA M., TANAKA I.
	Astron. Astrophys., 509A, 83-83 (2010)
	Optical and near-IR spectroscopy of candidate red galaxies in two z ~ 2.5 proto-clusters.
o	Table 2: <[DTD2010] MRC 0943-242 NNN> N=56 among (Nos 16-897), <[DTD2010] MRC 0943-242 HzRG> N=1, <[DTD2010] MRC 0943-242 LAENNNN> (Nos 381, 1141, 1618). Table 3: <[DTD2010] MRC 1138-262 NNN> N=33 among (Nos 90-905), <[DTD2010] JHHMMSS.ss+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DTF2002]
[DTF2002]	(Dallacasa+Tinti+Fanti+, 2002) (Not yet in Simbad)
Write:	<<[DTF2002] HHMM+DDd WN>> <<[DTF2002] HHMM+DDd WW>> <<[DTF2002] HHMM+DDd CeN>>
N:	101
Object:	Component (SIMBAD class: Radio = Radio Source)
Note:	Radio components of 28 B3 sources. See also [FPD2001b], [DFG2002].
Ref:	=2002A&A...389..115D
by	DALLACASA D. , TINTI S., FANTI C., FANTI R., GREGORINI L., STANGHELLINI C., VIGOTTI M.
	Astron. Astrophys., 389, 115-125 (2002)
	The B3-VLA CSS sample. II. VLBA images at 18 cm.
o	Figs, Table 2: <[DTF2002] HHMM+DDd WN>, <[DTF2002] HHMM+DDd CeN>, <[DTF2002] HHMM+DDdWW>, N=101.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DTH2012]
[DTH2012]	(De Boer+Tolstoy+Hill+, 2012)
Write:	<<[DTH2012] JHHMMSS.ss+DDMMSS.ss>>
N:	276283 (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	CTIO 4m MOSAIC II camera observations of covering the centre of the Fornax dwarf spheroidal galaxy.
in source:	NAME Fornax Dwarf Spheroidal
Ref:	=2012A&A...544A..73D
by	DE BOER T.J.L. , TOLSTOY E., HILL V., SAHA A., OLSZEWSKI E.W., MATEO M., STARKENBURG E., BATTAGLIA G., WALKER M.G.
	Astron. Astrophys., 544A, 73-73 (2012)
	The star formation and chemical evolution history of the Fornax dwarf spheroidal galaxy.
o	<[DTH2012] JHHMMSS.ss+DDMMSS.ss> N=276283
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DTH99]
[DTH99]	(Dominici+Teixeira+Harvath+, 1999)
Write:	<<[DTH99] AA NN-NNN>>
N:	506
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=506 reference stars for the 12 low-extinction fields (T.1) towards the Galactic Bulge. In the format 'AA NN-' represent the window (NN from 1 to 31) and 'NNN' a sequential counter number. See also [DHM99], objects coming from the same database of N=124976 objects.
in source:	NAME Galactic Bulge
Ref:	=1999A&AS..136..261D
by	DOMINICI T.P. , TEIXEIRA R., HORVATH J.E., MEDINA TANCO G.A., BENEVIDES-SOARES P.
	Astron. Astrophys., Suppl. Ser., 136, 261-267 (1999)
	Extension of Tycho catalog for low-extinction windows in the Galactic Bulge.
o	Table 3: <[DTH99] AA NN-NNN> N=506.
=E=	Catalogue in electronic form as J/A+AS/136/261
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DTJ80]
[DTJ80]	(Dufour+Talbot+Jensen+, 1980)= (D)
Write:	<<[DTJ80] R>>
N:	6
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Map in Fig.1
in source:	M 83 = NGC 5236
Ref:	=1980ApJ...236..119D
by	DUFOUR R.J. , TALBOT R.J.Jr, JENSEN E.B., SHIELDS G.A.
	Astrophys. J., 236, 119-134 (1980)
	M 83 II: spectral characteristics and chemical abundances of HII regions.
o	Table 1: <[DTJ80] R> (Nos I to VI)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DTM2008]
[DTM2008]	(De Mello+Torres-Flores+Mendes De Oliveira, 2008)
Write:	<<[DTM2008] NNA>>
N:	16+2
Object:	(Far UV) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	GALEX UV observations of the compact group of galaxies HCG 100.
in source:	HCG 100
Ref:	=2008AJ....135..319D
by	DE MELLO D.F. , TORRES-FLORES S., MENDES DE OLIVEIRA C.
	Astron. J., 135, 319-325 (2008)
	Searching for star formation outside galaxies: multiwavelength analysis of the intragroup medium of Hickson Compact Group 100.
o	Table 2: <[DTM2008] NNA> (Nos 1-16, 13A-13B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DTT2020]
[DTT2020]	(De La Fuente+Tafoya+Trinidad+, 2020)
Write:	<<[DTT2020] GLLL.lll+BB.bbb>>
N:	3
Object:	(mm) + Clump (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	VLA and OVRO observations of N=3 clumps in the ultracompact HII region GAL 043.89-00.78. Use of archival Spitzer (GLIMPSE, MIPSGAL) and ALMA data.
in source:	GAL 043.89-00.78
Ref:	=2020MNRAS.497.4436D
by	DE LA FUENTE E. , TAFOYA D., TRINIDAD M.A., PORRAS A., NIGOCHE-NETRO A., KEMP S.N., KURTZ S.E., FRANCO J., RODRIGUEZ-RICO C.A.
	Mon. Not. R. Astron. Soc., 497, 4436-4447 (2020)
	Ultracompact H II regions with extended emission: the case of G43.89-0.78 and its molecular environment.
o	Figs 4-5, Table 5: <[DTT2020] GLLL.lll+BB.bbb> (Nos G043.890-00.784, G043.899-00.786, G043.888-00.787).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DTV2016]
[DTV2016]	(Das+Tej+Vig+, 2016)
Write:	<<[DTV2016] S10 NN>> <<[DTV2016] EGO345 N>> <<[DTV2016] S10 Clump N>> <<[DTV2016] EGO345 Clump N>>
N:	19+8
Object:	YSO + Clump (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Search of N=14+5 YSOs and N=8 clumps in N=2 high-mass star-forming regions. Use of archival Spitzer GLIMPSE data.
in source:	[CPA2006] S10
in source:	EGO G345.99-0.02
Ref:	=2016AJ....152..152D
by	DAS S.R. , TEJ A., VIG S., GHOSH S.K., ISHWARA CHANDRA C.H.
	Astron. J., 152, 152-152 (2016)
	High-mass star formation toward southern infrared bubble S10.
o	Table 2, Fig. 5: <[DTV2016] S10 NN> (Nos 1-14), <[DTV2016] EGO345 N> (Nos 1-5). Table 4: <[DTV2016] S10 Clump N> (Nos 1-6), <[DTV2016] EGO345 Clump N> (Nos 7-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DTV2017]
[DTV2017]	(Das+Tej+Vig+, 2017) (Not yet in Simbad)
Write:	<<[DTV2017] Star N>> <<[DTV2017] Clump N>> <<[DTV2017] YSO NN>>
N:	5+5+93
Object:	* + Clump + YSO (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	GMRT 610 and 1300MHz observations of N=5 candidate ionizing stars, and N=5 cold dust clumps in the infrared dust bubble [CWP2007] CS 51. Use of Spitzer GLIMPSE and MIPSGAL data to identify N=93 YSOs towards the bubble. Use of archival 2MASS, Herschel and MALT90 survey data.
in source:	[CWP2007] CS 51
Ref:	=2017MNRAS.472.4750D
by	DAS S.R. , TEJ A., VIG S., LIU H.-L., LIU T., ISHWARA CHANDRA C.H., GHOSH S.K.
	Mon. Not. R. Astron. Soc., 472, 4750-4768 (2017)
	Infrared dust bubble CS51 and its interaction with the surrounding interstellar medium.
o	Fig. 4, Table 5: <[DTV2017] Star N> (Nos 1-5). Fig. 5, Table 6: <[DTV2017] Clump N> (Nos 1-5). Table A1: <[DTV2017] YSO NN> (Nos 1-93).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: dTZZ
dTZZ	(Di Tullio Zinn+Zinn)
*****	Avoid the usage of dTZZ, prefer [DZ2015]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Du
Du	(Dubout)= (Dub) = (Dubout)
Write:	<<Du NN>>
N:	81
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	OHP observations of HII regions in the Northern Milky Way.
Ref:	=1976A&AS...25...25D
by	DUBOUT-CRILLON R.
	Astron. Astrophys., Suppl. Ser., 25, 25-54 (1976)
	HII regions of the Northern Milky Way: medium large field photographic atlas and catalogue.
o	Table 1, col(1): numbering 'NNN' not used in SIMBAD
o	Table 1, col(2): <Du NN> N=81 among (Nos 1-88).
=E=	Catalogue in electronic form as <J/A+AS/25/25/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Dub
Dub	(Dubout) (Not yet in Simbad)
*****	Avoid the usage of Dub, prefer Du
Details on Acronym: Dubout
Dubout	(Dubout) (Not yet in Simbad)
*****	Avoid the usage of Dubout, prefer Du
Details on Acronym: Dufay
Dufay	(Dufay)
Write:	<<Cl Dufay N>>
N:	1
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Auth.:	DUFAY J.+
Details on Acronym: DUGRS
DUGRS	(Durham UKST Galaxy Redshift Survey)= DUKST
Write:	<<DUGRS FFF-NNN>>
N:	4412
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Radial velocities and magnitudes for all galaxies within the Durham/UKST Galaxy Redshift Survey. In the format, 'FFF' stands for N=60 UKST field numbers.
Ref:	=1998MNRAS.300..417R
by	RATCLIFFE A. , SHANKS T., PARKER Q.A., BROADBENT A., WATSON F.G., OATES A.P., COLLINS C.A., FONG R.
	Mon. Not. R. Astron. Soc., 300, 417-462 (1998)
	The Durham/UKST galaxy redshift survey - V. The catalogue.
o	<DUGRS FFF-NNN> N=4412.
=E=	Catalogue in electronic form as J/MNRAS/300/417
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DUKSKUS
DUKSKUS	(Dobashi+Uehara+Kandori Sakurai+Kaiden+Uemoto+Sato)
====>	Equivalent to: TGU
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DUKST
DUKST	(Durham UKST survey)
====>	Equivalent to: DUGRS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DUM2012]
[DUM2012]	(De Mello+Urrutia-Viscarra+Mendes De Oliveira+, 2012)
Write:	<<[DUM2012] HCG NNN NN>> <<[DUM2012] NGC NNNN NN>>
N:	14+35
Object:	Star Forming Region + (UV) (SIMBAD class: UV = UV-emission Source)
Note:	Gemini GMOS spectroscopy of N=12+2 star forming regions within the HI tails of HCG 92 and HCG 100. Use of GALEX FUV and NUV data for N=35 UV sources in the extended HI tails of six interacting systems.
in source:	HCG 92
in source:	HCG 100
in source:	NGC 2623
in source:	NGC 3079
in source:	NGC 3359
in source:	NGC 3627
in source:	NGC 3718
in source:	NGC 4656
Ref:	=2012MNRAS.426.2441D
by	DE MELLO D.F. , URRUTIA-VISCARRA F., MENDES DE OLIVEIRA C., TORRES-FLORES S., CARRASCO E.R., CYPRIANO E.
	Mon. Not. R. Astron. Soc., 426, 2441-2451 (2012)
	Star formation in HI tails: HCG 92, HCG 100 and six interacting systems.
o	Table 1: <[DUM2012] HCG NNN NN> N=14. Table 2: <[DUM2012] NGC NNNN NN> N=35.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DUO
DUO	(Disk Unseen Objects)
Write:	<<DUO N>>
N:	1
Object:	Poss. binary lens (SIMBAD class: LensingEv = (Micro)Lensing Event)
Ref:	=1995A&A...300L..17A
by	ALARD C. , MAO S., GUIBERT J.
	Astron. Astrophys., 300, 17-20 (1995)
	Object DUO 2: a new binary lens candidate ?
o	<DUO N> No. 2
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: DuRe
DuRe	(Duerbeck+Reipurth)
Write:	<<PN DuRe N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	DuRe 1 = PN G302.3-01.3
Ref:	=1990A&A...231L..11D
by	DUERBECK H.W. , REIPURTH B.
	Astron. Astrophys., 231, 11-14 (1990)
	We 21 : A WN 8 star in a planetary nebula.
o	We 21 = [W74] 21
o	<PN DuRe N> (No. 1).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: DV
DV	(Davoust+de Vaucouleurs)
Origin	of the Acronym: L (1996MNRAS.283..990T)
Details on Acronym: DV
DV	(De Vaucouleurs)= (DeV) = (Dev G) = (DVCG) = (G)
Write:	<<DV NN>>
N:	54
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Ref:	=1975SSS.....9..557D
by	DE VAUCOULEURS G.
	Stars and stellar systems., 9, 557-None (1975)
	Nearby groups of galaxies.
o	Galaxies and the Universe, 1975, Ed. Sandage A., Serie Stars and stellar systems, Vol. 9, chapter 14, p. 557-600.
o	<DV NN> (Nos 1-54).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: DV
DV	(Dunsink univ., Variable *)
Write:	<<*SV DV** NNN>>
N:	307
Object:	V* (SIMBAD class: Variable* = Variable Star)
in source:	Magellanic Clouds:LMC = LMC
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1974DunOP...1..193B
by	BUTLER C.J. , WAYMAN P.A.
	Dunsink Observatory, Dublin, Ireland - Publications, 1, 193-206 (1974)
	Identification of variable stars in the Magellanic Clouds.
o	Table I: <SV* DV NNN> (Nos 1-307)
Details on Acronym: [DV2005]
[DV2005]	(Durant+Van Kerkwijk, 2005)
Write:	<<[DV2005] A>>
N:	3
Object:	* (SIMBAD class: Star)
Note:	HST WFPC2 observations of the field around CXOU J010043.1-721134. 3 stars are found in the error circle of CXOU, the star X is proposed as counterpart. See also [DV2008].
Ref:	=2005ApJ...628L.135D
by	DURANT M. , VAN KERKWIJK M.H.
	Astrophys. J., 628, 135-138 (2005)
	Possible optical detection of the anomalous X-ray pulsar CXOU J010043.1-721134.
o	Table 1: <[DV2005] A> (Nos X, Y, Z).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DV2006]
[DV2006]	(Durant+Van Kerkwijk, 2006)
Write:	<<[DV2006] NN>> <<[DV2006] a>>
N:	27+8
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Magellan Clay telescope NIR observations of stars in the field around 1RXS J170849.0-400910 (N=27). N=8 stars are found around 1RXS J170849.0-400910 using archival VLT NACO data.
Ref:	=2006ApJ...648..534D
by	DURANT M. , VAN KERKWIJK M.H.
	Astrophys. J., 648, 534-540 (2006)
	The infrared counterpart to the magnetar 1RXS J170849.0-400910.
o	Table 3, Fig.3: <[DV2006] NN> (Nos 1-27). Table 4, Fig.4: <[DV2006] a> (Nos p-w).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DV2008]
[DV2008]	(Durant+Van Kerkwijk, 2008)
Write:	<<[DV2008] NN>>
N:	9
Object:	* (SIMBAD class: Star)
Note:	HST WFPC2 archives of the field around CXOU J010043.1-721134. See also [DV2005].
Ref:	=2008ApJ...680.1394D
by	DURANT M. , VAN KERKWIJK M.H.
	Astrophys. J., 680, 1394-1397 (2008)
	A search for the optical counterpart to the magnetar CXOU J010043.1-721134.
o	Fig.1: X, Y, Z = [DV2005] X, Y, Z.
o	Table 1, Fig.1: <[DV2008] NN> N=9 among (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DV59]
[DV59]	(Dolidze+Vyasovov, 1959)= (Dolidze)
Write:	<<[DV59] NNN>>
N:	125
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Ref:	=1959AbaOB..24....3D
by	DOLIDZE M.W. , WJASOWOW W.W.
	Byull. Abastumanskaya Astrofiz. Obs., 24, 3-5 (1959)
	The stars with H α-emission in the region around µ Cephei.
o	<[DV59] NNN> (Nos 1-125)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DV78]
[DV78]	(Dufour+Van Den Bergh, 1978)= (DF)
Write:	<<[DV78] DF N>>
N:	7
Object:	Feature (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Diffuse Features (DF in the format) in the inner jet of NGC 5128.
in source:	Cen A = NGC 5128
Ref:	=1978ApJ...226L..73D
by	DUFOUR R.J. , VAN DEN BERGH S.
	Astrophys. J., 226, 73-77 (1978)
	The inner structure of the optical jet in NGC 5128.
o	Table 2: <[DV78] DF N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DV98]
[DV98]	(De Blok+van der Hulst, 1998) (Not yet in Simbad)
Write:	<<[DV98] FNNN-N N-N>> <<[DV98] FNNN-VN N-N>> <<[DV98] UNNNN N-N>>
N:	43
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Table 1: N=43 HII regions in 11 galaxies (LSB format 'FNNN-N', VLSB format 'FNNN-VN' and UGC format 'UNNNN')
Ref:	=1998A&A...335..421D
by	DE BLOK W.J.G. , VAN DER HULST J.M.
	Astron. Astrophys., 335, 421-430 (1998)
	Star formation and the interstellar medium in low surface brightness galaxies. I. Oxygen abundances and abundance gradients in low surface brightness disk galaxies.
o	Table 1: <[DV98] FNNN-N N-N>, <[DV98] FNNN-VN N-N>, <[DV98] UNNNN N-N>, N=43.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DVC2012]
[DVC2012]	(Duronea+Vasquez+Cappa+, 2012)
Write:	<<[DVC2012] G289.49+00.15>>
N:	1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=1 radio source in the field of NGC 3503. Use of unpublished ATCA radio continuum data at 4800 and 8640MHz and of radio continuum SUMSS archival images at 843MHz.
in source:	NGC 3503
Ref:	=2012A&A...537A.149D
by	DURONEA N.U. , VASQUEZ J., CAPPA C.E., CORTI M., ARNAL E.M.
	Astron. Astrophys., 537A, 149-149 (2012)
	NGC 3503 and its molecular environment.
o	Fig. 7, Paragr. 3.2: <[DVC2012] G289.49+00.15> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DVC98]
[DVC98]	(Durouchoux+Vilhu+Corbel+, 1998)
Write:	<<[DVC98] N>>
N:	6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=6 radio-sources in the field of EXS 1737.9-2952. Maps in Figs 3, 5.
Ref:	=1998ApJ...507..781D
by	DUROUCHOUX P. , VILHU O., CORBEL S., WALLYN P., DWARAKANATH K.S., HUOVELIN J., ANANTHARAMAIAH K.R., GRINDLAY J., CHAPUIS C., PARK Y.-S., BALLY J., MAHONEY W.
	Astrophys. J., 507, 781-793 (1998)
	Multiwavelength observation of a new black hole candidate: EXS 1737.9-2952.
o	In Introduction, GRS 1741-2851 is Granat 1741.9-2853.
o	Table 2: <[DVC98] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DVCG
DVCG	(De Vaucouleurs)
*****	Avoid the usage of DVCG, prefer DV
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [DVG2015]
[DVG2015]	(Duronea+Vasquez+Gomez+, 2015)
Write:	<<[DVG2015] NN>>
N:	60
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	APEX LABOCA 870µm continuum observations of N=60 dust clumps around the bubble HII region Gum 31. Use of Spitzer GLIMPSE and SUMSS surveys.
in source:	GUM 31
Ref:	=2015A&A...582A...2D
by	DURONEA N.U. , VASQUEZ J., GOMEZ L., CAPPA C.E., FIRPO V., LOPEZ-CARABALLO C.H., RUBIO M.
	Astron. Astrophys., 582A, 2-2 (2015)
	870 µm continuum observations of the bubble-shaped nebula Gum 31.
o	Paragraph 2 standard star N207 11R not identified.
o	Table 1: <[DVG2015] NN> (Nos 1-60).
=E=	Catalogue in electronic form as <J/A+A/582/A2/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DVG98]
[DVG98]	(Donahue+Voit+Gioia+, 1998)= (D)
Write:	<<[DVG98] NN>>
N:	12
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	ASCA, ROSAT observations.
in source:	1E 1054.4-0321 = ClG 1054-0321
Ref:	=1998ApJ...502..550D
by	DONAHUE M. , VOIT G.M., GIOIA I., LUPPINO G., HUGHES J.P., STOCKE J.T.
	Astrophys. J., 502, 550-557 (1998)
	A very hot, high-redshift cluster of galaxies: more trouble for Ω_{0}=1.
o	Table 2: <[DVG98] NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DVH79]
[DVH79]	(Dufour+Van den Bergh+Harvel+, 1979)
Write:	<<[DVH79] NN>> <<[DVH79] Star A>>
N:	75+5
Object:	HII + * (SIMBAD class: HIIReg = HII Region)
Note:	N=75 HII regions in NGC 5128. N=5 reference stars (Nos A-E) around NGC 5128.
in source:	Cen A = NGC 5128
Ref:	=1979AJ.....84..284D
by	DUFOUR R.J. , VAN DEN BERGH S., HARVEL C.A., MARTINS D.H., SCHIFFER III F.H., TALBOT R.J.Jr, TALENT D.L., WELLS D.C.
	Astron. J., 84, 284-301 (1979)
	Picture processing analysis of the optical structure of NGC 5128 (Centaurus A).
o	Fig.4: D and E (and E1-E2) components, A1-A5 not in SIMBAD.
o	Fig.8, Table II: <[DVH79] NN> (Nos 1-75), <[DVH79] Star A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DVR2000]
[DVR2000]	(De Breuck+Van Breugel+Rottgering+, 2000)= (MP) = (TN) = (WN)
Write:	<<[DVR2000] WN JHHMM+DDMMA>> <<[DVR2000] TN JHHMM+DDMM>> <<[DVR2000] MP JHHMM+DDMM>>
N:	343+268+58
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table a1: 'WN' = WN-NVSS sources. Table a2: 'TN' = TXS-NVSS sources. Table a3: 'MP' = MRC-PMN sources.
Ref:	=2000A&AS..143..303D
by	DE BREUCK C. , VAN BREUGEL W., ROETTGERING H.J.A., MILEY G.
	Astron. Astrophys., Suppl. Ser., 143, 303-333 (2000)
	A sample of 669 ultra steep spectrum radio sources to find high redshift radio galaxies.
o	in ref list COLEMAN 1985AJ.....90.1431C instead of AJ.90.8, DE RUITER 1977A&AS...28..211D instead of A&A.28.211, FANAROFF 1974MNRAS.167p.. 31F instead of FARANOFF MNRAS.167.31
o	Table a1: <[DVR2000] WN JHHMM+DDMM> N=343. Table a2: <[DVR2000] TN JHHMM+DDMM> N=268. Table a3: <[DVR2000] MP JHHMM+DDMM> N=58.
=E=	Catalogue in electronic form as J/A+AS/143/303
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DVR2021]
[DVR2021]	(Di Gennaro+Van Weeren+Rudnick+, 2021)= ([DVR2021a])
Write:	<<[DVR2021] NN>>
N:	10
Object:	Radio G (SIMBAD class: RadioG = Radio Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLA 1-4 GHz continuum observations of N=10 radio galaxies in the field of the galaxy cluster CIZA J2242.8+5301.
in source:	CIZA J2242.8+5301
Ref:	=2021ApJ...911....3D
by	DI GENNARO G. , VAN WEEREN R.J., RUDNICK L., HOEFT M., BRUGGEN M., RYU D., ROTTGERING H.J.A., FORMAN W., STROE A., SHIMWELL T.W., KRAFT R.P., JONES C., HOANG D.N.
	Astrophys. J., 911, 3-3 (2021)
	Downstream depolarization in the Sausage Relic: a 1-4 GHz very large array study.
o	Fig. 2, Table 2: <[DVR2021] NN> (Nos 1-10).
o	Sources from figures 3 and 4 are not in SIMBAD.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DVR2021a]
[DVR2021a]	(Di Gennaro+Van Weeren+Rudnick+, 2021)
*****	Avoid the usage of [DVR2021a], prefer [DVR2021]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DVR2021b]
[DVR2021b]	(Daddi+Valentino+Rich+, 2021)
Write:	<<[DVR2021b] RO-1001>> <<[DVR2021b] RO-1001 A>> <<[DVR2021b] RO-1001 nebula>> <<[DVR2021b] RO-1001 filament N>>
N:	1+4+1+3
Object:	Group of G + G + Em. Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Keck KCWI and NOEMA observations of N=1 group of galaxies, N=4 galaxies in this group, N=1 Lyman alpha nebula, N=3 Lyman alpha filaments. Use of publicly available ALMA band 7 data.
Ref:	=2021A&A...649A..78D
by	DADDI E. , VALENTINO F., RICH R.M., NEILL J.D., GRONKE M., O'SULLIVAN D., ELBAZ D., BOURNAUD F., FINOGUENOV A., MARCHAL A., DELVECCHIO I., JIN S., LIU D., STRAZZULLO V., CALABRO A., COOGAN R., D'EUGENIO C., GOBAT R., KALITA B.S., LAURSEN P., MARTIN D.C., PUGLISI A., SCHINNERER E., WANG T.
	Astron. Astrophys., 649A, 78-78 (2021)
	Three Lyman-α-emitting filaments converging to a massive galaxy group at z = 2.91: discussing the case for cold gas infall.
o	<[DVR2021b] RO-1001> N=1. <[DVR2021b] RO-1001 nebula> N=1. Fig. 1: <[DVR2021b] RO-1001 filament N> (Nos 1-3). Fig. 2, Table 1: <[DVR2021b] RO-1001 A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DVS2002]
[DVS2002]	(De Breuck+Van Breugel+Stanford+, 2002)
Write:	<<[DVS2002] WN JHHMM+DDMM A(opt)>> <<[DVS2002] WN JHHMM+DDMM A(IR)>> <<[DVS2002] TN JHHMM+DDMM A(opt)>> <<[DVS2002] TN JHHMM+DDMM A(IR)>> <<[DVS2002] MP JHHMM+DDMM A(IR)>>
N:	129
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Offset stars observed in opt. or in IR for the 128 [DVR2000] radio-sources studied.
Ref:	=2002AJ....123..637D
by	DE BREUCK C. , VAN BREUGEL W., STANFORD S.A., ROETTGERING H., MILEY G., STERN D.
	Astron. J., 123, 637-677 (2002)
	Optical and near-infrared imaging of ultra-steep-spectrum radio sources: the K-z diagram of radio-selected and optically selected galaxies.
o	In table 5, WN J0837-1053 is a misprint for TN J0837-1053; in table 6, TN J0859-1510 is a misprint for TN J0856-1510.
o	Table 6, Fig.12: <[DVS2002] WN JHHMM+DDMM A(IR)>, <[DVS2002] WN JHHMM+DDMM A(opt), <[DVS2002] TN JHHMM+DDMM A(IR)>, <[DVS2002] TN JHHMM+DDMM A(opt), <[DVS2002] MP JHHMM+DDMM A(IR)>, N=129.
=E=	Catalogue in electronic form as J/AJ/123/637
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DVS2018]
[DVS2018]	(Dopita+Vogt+Sutherland+, 2018) (Not yet in Simbad)
Write:	<<[DVS2018] PNN>>
N:	20
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Note:	ANU 2.3m telescope WiFeS integral-field spectroscopy of N=20 shocked clouds in the field of the supernova remnant N132D in the LMC. Use of archival HST ACS images.
in source:	LHA 120-N 132D
Ref:	=2018ApJS..237...10D
by	DOPITA M.A. , VOGT F.P.A., SUTHERLAND R.S., SEITENZAHL I.R., RUITER A.J., GHAVAMIAN P.
	Astrophys. J., Suppl. Ser., 237, 10-10 (2018)
	Shocked interstellar clouds and dust grain destruction in the LMC supernova remnant N132D.
o	Table 1: <[DVS2018] PNN> (Nos P1-P20).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DVS99]
[DVS99]	(Donahue+Voit+Scharf+, 1999)
Write:	<<[DVS99] NN>>
N:	23
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	ASCA, Keck and ROSAT observations of the ClG 1E 1137.5+6625.
in source:	1E 1137.0+6625
Ref:	=1999ApJ...527..525D
by	DONAHUE M. , VOIT G.M., SCHARF C.A., GIOIA I.M., MULLIS C.R., HUGHES J.P., STOCKE J.T.
	Astrophys. J., 527, 525-None (1999)
	The second most distant cluster of galaxies in the extended medium sensitivity survey.
o	p. 532 : ClG AX 2019 = AX J2019+114
o	Fig.2, Table 3: <[DVS99] NN> (Nos 1-23).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DVT2021]
[DVT2021]	(Dalessandro+Varri+Tiongco+, 2021)= (LISCA) = ([DVT2021a])
Write:	<<[DVT2021] LISCA I>> <<[DVT2021] N N>>
N:	1+3
Object:	Cluster of * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	TNG HARPS-N and GIANO-B observations of N=1 substructured stellar system and N=3 star clusters. LISCA stands for Lively Infancy of Star Clusters and Associations. Use of Gaia EDR3 data.
Ref:	=2021ApJ...909...90D
by	DALESSANDRO E. , VARRI A.L., TIONGCO M., VESPERINI E., FANELLI C., MUCCIARELLI A., ORIGLIA L., BELLAZZINI M., SARACINO S., OLIVA E., SANNA N., FABRIZIO M., LIVERNOIS A.
	Astrophys. J., 909, 90-90 (2021)
	First phase space portrait of a hierarchical stellar structure in the Milky Way.
o	<[DVT2021] LISCA I> N=1. Fig. 1, Table 1: <[DVT2021] N N> (Nos N 1-N 3).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [DVT2021a]
[DVT2021a]	(Dalessandro+Varri+Tiongco+, 2021)= (LISCA)
*****	Avoid the usage of [DVT2021a], prefer [DVT2021]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [DVT2021b]
[DVT2021b]	(Dage+Vowell+Thygesen+, 2021)
Write:	<<[DVT2021b] NNNNNULXN>>
N:	12
Object:	Poss. ULX (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	N=12 ultraluminous X-ray (ULX) candidates in four edge-on spiral galaxies. Use of Chandra and XMM-Newton archival data.
in source:	NGC 891
in source:	NGC 3556
in source:	NGC 4157
in source:	NGC 7331
Ref:	=2021MNRAS.508.4008D
by	DAGE K.C. , VOWELL N., THYGESEN E., BAHRAMIAN A., HAGGARD D., KOVLAKAS K., KUNDU A., MACCARONE T.J., STRADER J., URQUHART R., ZEPF S.E.
	Mon. Not. R. Astron. Soc., 508, 4008-4016 (2021)
	Ultraluminous X-ray sources in seven edge-on spiral galaxies.
o	Table 1: <[DVT2021b] NNNNNULXN> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DVZ2014]
[DVZ2014]	(Duffau+Vivas+Zinn+, 2014)
Write:	<<[DVZ2014] NNN>>
N:	25
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Note:	KPNO WIYN, La Silla 1.5 and 3.6m and CTIO 4m and 1.5m observations of 25 RR Lyrae stars in the Virgo stellar stream.
in source:	NAME Virgo Stellar Stream
Ref:	=2014A&A...566A.118D
by	DUFFAU S. , VIVAS A.K., ZINN R., MENDEZ R.A., RUIZ M.T.
	Astron. Astrophys., 566A, 118-118 (2014)
	A comprehensive view of the Virgo stellar stream.
o	Table 6: <[DVZ2014] NNN> N=25 among (Nos 716-757).
=E=	Catalogue in electronic form as <J/A+A/566/A118/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Dw
Dw	(Dwarf galaxy)
*****	Avoid the usage of Dw, prefer [B97b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Dw
Dw	(Dwarf G)
*****	Avoid the usage of Dw, prefer [C83]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Dw
Dw	(Dwingeloo obs.)= (DwO)
Write:	<<Dw HHMM+DD>>
N:	188
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Ref:	=1967BAN....19..201D
by	DAVIS M.M.
	Bull. Astron. Inst. Netherlands, 19, 201-226 (1967)
	A 1417 MHz search for radio sources having a flux excess at short wavelengths.
o	Table 6: <Dw HHMM+DD> N=188.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Dw
Dw	(Dwingeloo obs.)
*****	Avoid the usage of Dw, prefer Dwingeloo
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DW74]
[DW74]	(Downes+Wilson, 1974)
Write:	<<[DW74] H2CO Maser>>
N:	1
Object:	H2CO Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	Effelsberg observations. Search for H2CO emission near NGC 7538.
Ref:	=1974ApJ...191L..77D
by	DOWNES D. , WILSON T.L.
	Astrophys. J., 191, 77-78 (1974)
	Formaldehyde line emission at 4.8GHz near NGC 7538.
o	<[DW74] H2CO Maser> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DW81]
[DW81]	(Dreher+Welch, 1981)
Write:	<<[DW81] H2O Maser N>>
N:	3
Object:	H2O Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	See also [GBW85] and [BMW93]
in source:	W 3:W 3(OH) = W 3(OH)
Ref:	=1981ApJ...245..857D
by	DREHER J.W. , WELCH W.J.
	Astrophys. J., 245, 857-865 (1981)
	Discovery of shell structure in the ultracompact H II region W3(OH).
o	In table 2, the digit 3 is forgotten for the third maser (see Fig.3).
o	Table 2: <[DW81] H2O Maser N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DW98]
[DW98]	(Dietrich+Wagner, 1998)
Write:	<<[DW98] NN>>
N:	16
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Components of NGC 1068. See also [EFK91]
in source:	NGC 1068
Ref:	=1998A&A...338..405D
by	DIETRICH M. , WAGNER S.J.
	Astron. Astrophys., 338, 405-412 (1998)
	Kinematics of the narrow-line region of NGC 1068.
o	Table 1: <[DW98] NN> (Nos 1-16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DWA2016]
[DWA2016]	(Decarli+Walter+Aravena+, 2016)
Write:	<<[DWA2016] NN>> <<[DWA2016] ID.NN>> (not recognised by Simbad, but found in literature)
N:	11
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ALMA CO line observations of N=11 high-redshift galaxies. Use of the ALMA SPECtroscopic Survey in the Hubble Ultra-Deep Field (ASPECS). Use of archival HST (ACS and NICMOS) images. See also [WDA2016] and [ADW2016].
Ref:	=2016ApJ...833...70D
by	DECARLI R. , WALTER F., ARAVENA M., CARILLI C., BOUWENS R., DA CUNHA E., DADDI E., ELBAZ D., RIECHERS D., SMAIL I., SWINBANK M., WEISS A., BACON R., BAUER F., BELL E.F., BERTOLDI F., CHAPMAN S., COLINA L., CORTES P.C., COX P., GONZALEZ-LOPEZ J., INAMI H., IVISON R., HODGE J., KARIM A., MAGNELLI B., OTA K., POPPING G., RIX H.-W., SARGENT M., VAN DER WEL A., VAN DER WERF P.
	Astrophys. J., 833, 70-70 (2016)
	The ALMA spectroscopic survey in the Hubble Ultra Deep Field: molecular gas reservoirs in high-redshift galaxies.
o	Tables 1-2: <[DWA2016] NN> (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DWA2018]
[DWA2018]	(Durret+Wakamatsu+Adami+, 2018)= (OPH)
Write:	<<[DWA2018] OPH JHHMMSS.ss+DDMMSS>>
N:	2818
Object:	G (SIMBAD class: Galaxy)
Note:	CFHT MegaCam photometric observations of N=2818 galaxies in the Ophiuchus cluster.
in source:	NAME Oph Cluster
Ref:	=2018A&A...613A..20D
by	DURRET F. , WAKAMATSU K., ADAMI C., NAGAYAMA T., OMEGA MULEKA MWEWA MWABA J.M.
	Astron. Astrophys., 613A, 20-20 (2018)
	The optical properties of galaxies in the Ophiuchus cluster.
o	Table B.1: <[DWA2018] OPH JHHMMSS.ss+DDMMSS> N=2818.
=E=	Catalogue in electronic form as J/A+A/613/A20
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DWB
DWB	(Dickel+Wendker+Bieritz)
Write:	<<DWB NNN>>
N:	193
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Ref:	=1969A&A.....1..270D
by	DICKEL H.R. , WENDKER H.J., BIERITZ J.H.
	Astron. Astrophys., 1, 270-280 (1969)
	The Cygnus X region. V. Catalogue and distances of optically visible H II regions.
o	Table :<DWB NNN> (Nos 1-193)
Origin	of the Acronym: L (1974Ap&SS..27....3M)
Details on Acronym: [DWB80]
[DWB80]	(Downes+Wilson+Bieging+, 1980)
Write:	<<[DWB80] LLL.lll+B.bbb>>
N:	262
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1980A&AS...40..379D
by	DOWNES D. , WILSON T.L., BIEGING J., WINK J.
	Astron. Astrophys., Suppl. Ser., 40, 379-394 (1980)
	H110α and H2CO survey of galactic radio sources.
o	Table II: <[DWB80] LLL.lll+B.bbb> N=262
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DWC2011]
[DWC2011]	(Dong+Wang+Cotera+, 2011)
Write:	<<[DWC2011] NNNa>>
N:	165+2
Object:	Em. Obj. (SIMBAD class: EmObj = Emission Object)
Stat:	is completely incorporated in Simbad
Note:	N=167 Paschen-α emitting candidates, from the HST/NICMOS Paschen-α survey of the Galactic Centre.
in source:	NAME Galactic Center
Ref:	=2011MNRAS.417..114D
by	DONG H. , WANG Q.D., COTERA A., STOLOVY S., MORRIS M.R., MAUERHAN J., MILLS E.A., SCHNEIDER G., CALZETTI D., LANG C.
	Mon. Not. R. Astron. Soc., 417, 114-135 (2011)
	Hubble Space Telescope Paschen α survey of the Galactic Centre: data reduction and products.
o	Table 3: <[DWC2011] NNN> (Nos 1-152).
Ref:	=2012MNRAS.425..884D
by	DONG H. , WANG Q.D., MORRIS M.R.
	Mon. Not. R. Astron. Soc., 425, 884-906 (2012)
	A multiwavelength study of evolved massive stars in the Galactic Centre.
o	Table 2: <[DWC2011] NNNa> (Nos 122a-b, 153-165) added.
=E=	Catalogue in electronic form as J/MNRAS/417/114
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DWC2014]
[DWC2014]	(Decarli+Walter+Carilli+, 2014)
Write:	<<[DWC2014] ID.NN>> <<[DWC2014] ID.CN>>
N:	21+5
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	IRAM PdBI 3mm continuum and CO line observations of N=21+5 galaxies in the Hubble Deep Field North (HDF-N). Use of HST WFPC3 archival data of the HDFN. See also [WDS2014].
in source:	NAME HDFN
Ref:	=2014ApJ...782...78D
by	DECARLI R. , WALTER F., CARILLI C., RIECHERS D., COX P., NERI R., ARAVENA M., BELL E., BERTOLDI F., COLOMBO D., DA CUNHA E., DADDI E., DICKINSON M., DOWNES D., ELLIS R., LENTATI L., MAIOLINO R., MENTEN K.M., RIX H.-W., SARGENT M., STARK D., WEINER B., WEISS A.
	Astrophys. J., 782, 78 (2014)
	A molecular line scan in the Hubble Deep Field North.
o	Table 2: <[DWC2014] ID.NN> (Nos ID.1-ID.21). Table 4: <[DWC2014] ID.CN> (Nos ID.C1-ID.C5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DWD2006]
[DWD2006]	(De Mello+Wadadekar+Dahlen+, 2006)
Write:	<<[DWD2006] N>>
N:	9
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 images of 9 luminous objects found in the UV-selected sample.
Ref:	=2006AJ....131..216D
by	DE MELLO D.F. , WADADEKAR Y., DAHLEN T., CASERTANO S., GARDNER J.P.
	Astron. J., 131, 216-225 (2006)
	Star-forming galaxies at intermediate redshifts: morphology, ages, and sizes.
o	Fig.16: <[DWD2006] N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DWF
DWF	(Deeper, Wider, Faster program)
Write:	<<DWF YYaNNNN>> <<DWF YYaa>> <<DWF JHHMMSS.sss+DDMMSS.sss>>
Object:	Opt. Transient (SIMBAD class: Transient = Transient Event)
Note:	The Deeper, Wider, Faster program (DWF) searches for optical transients. For more information, visit: https://dwfprogram.wixsite.com/home Only the first references are listed here.
Ref:	=2017ATel10072....1A
by	ANDREONI I. , COOKE J., PRITCHARD T.A., SPIEWAK R., PLANT K., MESTRIC U., RYDER S., ABBOTT T., ALLEN R., ANDERSON G., ASHER A., BAGLIO M.C., BANNISTER K., BELL M., BERNARD S., BHANDARI S., CALEB M., CAMPANA S., COWARD D., CURTIN C., D'AVANZO P., DEVLIN J.F., FARAH W., FLUKE C., FLYNN C., FORAN G., FUGAZZA D., GAWIN B., HEGARTY S., HODGSON R., HODGSON S., HORST J., HOWELL E., HUSSAINI I., JACOBS C., KO M., KOTZE M., LIEN A., MEADE B., MELANDRI A., MISZALSKI B., MOLLER A., MURPHY M.T., NANAYAKKARA T., O'NEILL M., OSLOWSKI S., PENG B., PETROFF E., REST A., ROBERT F., SHARA M., TUCKER B., VALDES F., VOHL D.
	The Astronomer's Telegram, 10072, 1 (2017)
	Discovery of 4 possible supernovae during the "Deeper, Wider, Faster" program observations.
o	<DWF17aNNNN> N=4.
Ref:	=2020MNRAS.491.5852A
by	ANDREONI I. , COOKE J., WEBB S., REST A., PRITCHARD T., CALEB M., CHANG S.-W., FARAH W., LIEN A., MOLLER A., RAVASIO M.E., ABBOTT T.M.C., BHANDARI S., CUCCHIARA A., FLYNN C., JANKOWSKI F., KEANE E.F., MORIYA T.J., ONKEN C.A., PARTHASARATHY A., PRICE D.C., PETROFF E., RYDER S., VOHL D., WOLF C.
	Mon. Not. R. Astron. Soc., 491, 5852-5866 (2020)
	Probing the extragalactic fast transient sky at minute time-scales with DECam.
o	<DWFYYaa> N=10 among (15a, 17a-17x, 17ao-17ax).
Ref:	=2020MNRAS.498.3077W
by	WEBB S. , LOCHNER M., MUTHUKRISHNA D., COOKE J., FLYNN C., MAHABAL A., GOODE S., ANDREONI I., PRITCHARD T., ABBOTT T.M.C.
	Mon. Not. R. Astron. Soc., 498, 3077-3094 (2020)
	Unsupervised machine learning for transient discovery in deeper, wider, faster light curves.
o	Tables 2+4+5: <DWF JHHMMSS.sss+DDMMSS.sss> N=7+6+10.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DWG95]
[DWG95]	(Driver+Windhorst+Griffiths, 1995)= (HST) = (MDS)
Write:	<<[DWG95] NNN>>
N:	144
Object:	G (SIMBAD class: Galaxy)
Note:	HST WFPC2 Medium Deep Survey
Ref:	=1995ApJ...453...48D
by	DRIVER S.P. , WINDHORST R.A., GRIFFITHS R.E.
	Astrophys. J., 453, 48-64 (1995)
	The contribution of late-type/irregulars to the faint galaxy counts from Hubble Space Telescope medium deep survey images.
o	<[DWG95] NNN> (Nos 1-144)
=E=	Catalogue in electronic form as J/ApJ/453/48
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DWH
DWH	(Dahlem+Weaver+Heckman)
Write:	<<DWH NGC NNNN NN>> <<DWH M 82 NN>>
N:	47+7
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT PSPC and HRI, ASCA observations. X-ray point sources in 4 galaxies.
in source:	NGC 55
in source:	NGC 253
in source:	NGC 4631
in source:	M 82 = NGC 3034
Ref:	=1998ApJS..118..401D
by	DAHLEM M. , WEAVER K.A., HECKMAN T.M.
	Astrophys. J., Suppl. Ser., 118, 401-453 (1998)
	An X-ray minisurvey of nearby edge-on starburst galaxies. I. The data.
o	Table 8: regions are 'geometrical areas' not objects.
o	Fig.7: <DWH NGC 55 N> (Nos 1-8). Fig.10: <DWH NGC 253 NN> (Nos 1-18). Fig.13: <DWH M 82 NN> (Nos 1-17). Fig.19: <DWH NGC 4631 N> (Nos 1-4).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Dwingeloo
Dwingeloo	(Dwingeloo obs.)= (Dw)
Write:	<<Dwingeloo N>> <<Dwingeloo LLL.l+B.b>>
N:	2+6
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=2 galaxies, Dwingeloo 1 and 2, were first identified. Dwingeloo 2 was identified by Verheijen, 1995, private communication, cited by 1995AJ....110.1584K. N=6 galaxies, 'Dwingeloo LLL.l+B.b', were added later, with Dwingeloo 138.5-0.1 = Dwingeloo 1.
Ref:	=1994Natur.372...38B
by	BURSTEIN D.
	Nature, 372, 38-None (1994)
	Unveiling a new galaxy.
o	New galaxy = 'Dwingeloo 1'
Ref:	=1995AJ....110.1584K
by	KRISMER M. , TULLY R.B., GIOIA I.M.
	Astron. J., 110, 1584-1587 (1995)
	IC 342/Maffei group of galaxies and distances for two of its members.
o	MB 1 = [MB95] 1
o	<Dwingeloo 2>
Ref:	=1998AJ....115..584H
by	HENNING P.A. , KRAAN-KORTEWEG R.C., RIVERS A.J., LOAN A.J., LAHAV O., BURTON W.B.
	Astron. J., 115, 584-591 (1998)
	Galaxies discovered behind the Milky Way by the Dwingeloo obscured galaxies survey.
o	Table 1: <Dwingeloo LLL.l+B.b> N=5
Ref:	=1999PASA...16...48R
by	RIVERS A.J. , HENNING P.A., KRAAN-KORTEWEG R.C.
	Publications - Astron. Soc. Australia, 16, 48-52 (1999)
	Galaxies detected by the Dwingeloo obscured galaxies survey.
o	<Dwingeloo LL.l+B.b> N=3.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DWM2010]
[DWM2010]	(Demarco+Wilson+Muzzin+, 2010)
Write:	<<[DWM2010] NNNNNNN>>
N:	22+19+34
Object:	G (SIMBAD class: Galaxy)
Note:	Keck I LRIS spectroscopic observations of galaxies in the field of three galaxy clusters.
in source:	SpARCS J161315+564930
in source:	SpARCS J161641+554513
in source:	SpARCS J161037+552417
Ref:	=2010ApJ...711.1185D
by	DEMARCO R. , WILSON G., MUZZIN A., LACY M., SURACE J., YEE H.K.C., HOEKSTRA H., BLINDERT K., GILBANK D.
	Astrophys. J., 711, 1185-1197 (2010)
	Spectroscopic confirmation of three red-sequence selected galaxy clusters at z = 0.87, 1.16, and 1.21 from the SpARCS survey.
o	Table 1: <SpARCS JHHMMSS+DDMMSS> N=3. Tables 2-4: <[DWM2010] NNNNNNN> N=22+19+34 among (Nos 708779-4000032).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DWM2014]
[DWM2014]	(Degenaar+Wijnands+Miller, 2014)
Write:	<<[DWM2014] N>>
N:	8
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton EPIC observations N=8 X-ray sources in the field of SAX J2224.9+5421.
in source:	SAX J2224.9+5421
Ref:	=2014ApJ...787...67D
by	DEGENAAR N. , WIJNANDS R., MILLER J.M.
	Astrophys. J., 787, 67 (2014)
	The quiescent counterpart of the peculiar X-ray burster SAX J2224.9+5421.
o	Table 1: <[DWM2014] N> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DWN2015]
[DWN2015]	(Durret+Wakamatsu+Nagayama+, 2015) (Not yet in Simbad)
Write:	<<[DWN2015] OPH JHHMMSS.ss+DDMMSS>>
N:	162+65
Object:	G (SIMBAD class: Galaxy)
Note:	CFHT Megacam, VLT FORS2, SOAR SOI observations of N=162+65 galaxies in the field of the Ophiuchus galaxy cluster.
in source:	NAME Ophiuchus Cluster
Ref:	=2015A&A...583A.124D
by	DURRET F. , WAKAMATSU K., NAGAYAMA T., ADAMI C., BIVIANO A.
	Astron. Astrophys., 583A, 124-124 (2015)
	Ophiuchus: An optical view of a very massive cluster of galaxies hidden behind the Milky Way.
o	Tables A.1-A.2: <[DWN2015] OPH JHHMMSS.ss+DDMMSS> N=162+65.
=E=	Catalogue in electronic form as J/A+A/583/A124
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DWN2020]
[DWN2020]	(Drake+Walter+Novak+, 2020)
Write:	<<[DWN2020] LAE 3>> <<[DWN2020] SRC 6>>
N:	1+1
Object:	LAE + ? (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT MUSE observations of N=1 Lyman α emitter and N=1 other source in the field of the quasar BR B1202-0725. Use of HST, ALMA and MUSE archival data. See also [CRW2013].
Ref:	=2020ApJ...902...37D
by	DRAKE A.B. , WALTER F., NOVAK M., FARINA E.P., NEELEMAN M., RIECHERS D., CARILLI C., DECARLI R., MAZZUCCHELLI C., ONOUE M.
	Astrophys. J., 902, 37-37 (2020)
	The ionized- and cool-gas content of the BR1202-0725 system as seen by MUSE and ALMA.
o	Fig. 1, Table 2: <[DWN2020] LAE 3> N=1, <[DWN2020] SRC 6> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DWN2021]
[DWN2021]	(Dunne+Webb+Noble+, 2021)
Write:	<<[DWN2021] XMM-CON>> <<[DWN2021] ES1-CONN>> <<[DWN2021] CDFS-CONN>>
N:	30
Object:	BCG (SIMBAD class: BrightestCG = Brightest Galaxy in a Cluster (BCG))
Stat:	is completely incorporated in Simbad
Note:	ALMA bands 3, 4, 5 CO(2-1) observations of N=30 brightest cluster galaxies (BCGs) over 0.2 ≤ z ≤ 1.2, as part of the Spitzer Adaptation of the Red-Sequence Cluster Survey (SpARCS). ES1 in the format stands for SWIRE fields ELAIS-S1. XMM in the format stands for XMM-LSS.
Ref:	=2021ApJ...909L..29D
by	DUNNE D.A. , WEBB T.M.A., NOBLE A., LIDMAN C., SHIPLEY H., MUZZIN A., WILSON G., YEE H.K.C.
	Astrophys. J., 909L, 29-29 (2021)
	A CO Survey of SpARCS star-forming brightest cluster galaxies: evidence for uniformity in BCG molecular gas processing across cosmic time.
o	Table 1: <[DWN2021] XMM-CON> (Nos 1-8), <[DWN2021] ES1-CONN> N=9 among (Nos 1-10), <[DWN2021] CDFS-CONN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DwO
DwO	(Dwingeloo Obs.)
*****	Avoid the usage of DwO, prefer Dw
Origin	of the Acronym: L (1977A&A....60..233I)
Details on Acronym: [DWS2012]
[DWS2012]	(Downes+Welch+Scott+, 2012)= (AzTEC/COSMOS) = (AzTEC/GN) = (AzTEC/LH) = (AzTEC/SXDF) = (AzTEC/GS)
Write:	<<[DWS2012] AzTEC/COSMOS NN>> <<[DWS2012] AzTEC/GN NN>> <<[DWS2012] AzTEC/LH NN>> <<[DWS2012] AzTEC/SXDF NN>> <<[DWS2012] AzTEC/GS NN.N>>
N:	50+40+95+65+57
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	New reduction of ASTE and JCMT AzTEC data in the COSMOS, Lockman Hole, SXDF, GOODS (North and South) fields. See also AzTEC.
in source:	NAME COSMOS Field
in source:	NAME GOODS North Field
in source:	NAME Lockman Hole
in source:	NAME SXDF
in source:	NAME GOODS South Field
Ref:	=2012MNRAS.423..529D
by	DOWNES T.P. , WELCH D., SCOTT K.S., AUSTERMANN J., WILSON G.W., YUN M.S.
	Mon. Not. R. Astron. Soc., 423, 529-542 (2012)
	Calculating the transfer function of noise removal by principal component analysis and application to AzTEC deep-field observations.
o	Table 1, col(1): <AzTEC JHHMMSS.ss+DDMMSS.s> N=50 = Table 1, col(2): <[DWS2012] AzTEC/COSMOS NN> (Nos 1-50). Table 2, col(1): <AzTEC JHHMMSS.ss+DDMMSS.s> N=40 = Table 2, col(2): <[DWS2012] AzTEC/GN NN> (Nos 1-40). Table 3, col(1): <AzTEC JHHMMSS.ss+DDMMSS.s> N=95 = Table 3, col(2): <[DWS2012] AzTEC/LH NN> (Nos 1-95). Table 4, col(1): <AzTEC JHHMMSS.ss+DDMMSS.s> N=65 = Table 4, col(2): <[DWS2012] AzTEC/SXDF NN> (Nos 1-65). Table 5, col(1): <AzTEC JHHMMSS.ss+DDMMSS.s> N=57 = Table 5, col(2): <[DWS2012] AzTEC/GS NN.N> (Nos 1-2, 2.1-2.2, 3-55).
=E=	Catalogue in electronic form as J/MNRAS/423/529
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DWS2016]
[DWS2016]	(De Blok+Walter+Smith+, 2016) (Not yet in Simbad)
Write:	<<[DWS2016] {M\|N}N>>
N:	4+3
Note:	SOFIA observations of N=4+3 star forming regions, respectively in M 101 and NGC 6946.
in source:	NGC 5457 = M 101
in source:	NGC 6946
Ref:	=2016AJ....152...51D
by	DE BLOK W.J.G. , WALTER F., SMITH J.-D., HERRERA-CAMUS R., BOLATTO A.D., REQUENA-TORRES M.A., CROCKER A.F., CROXALL K.V., KENNICUTT R.C., KODA J., ARMUS L., BOQUIEN M., DALE D., KRECKEL K., MEIDT S.
	Astron. J., 152, 51-51 (2016)
	Comparing [C II] , HI, and CO dynamics of nearby galaxies.
o	Fig. 3, Table 2: <[DWS2016] AN> (Nos M1-M4, N1-N3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DWS84]
[DWS84]	(Danks+Wamsteker+Shaver+, 1984)
Write:	<<[DWS84] GLLL.ll+B.bb>> <<[DWS84] IRS NN>> <<[DWS84] Cluster N>>
N:	11+72+2
Object:	(Rad) + (IR) + Cluster of * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Radio and IR observations of a region in the direction l=305deg, b=0.2. 11 radio-sources are found, 72 IR sources of which many are members of two new galactic clusters.
Ref:	=1984A&A...132..301D
by	DANKS A.C. , WAMSTEKER W., SHAVER P.A., RETALLACK D.S.
	Astron. Astrophys., 132, 301-311 (1984)
	A near-infrared study of the region l = 305.
o	Table 1: <[DWS84] GLLL.ll+B.bb> N=11. Table 2: <[DWS84] IRS NN> (Nos 1-72). Text: : <[DWS84] Cluster N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DWS97]
[DWS97]	(Downes+Webbink+Shara, 1997)
Write:	<<[DWS97] CCC N>>
N:	157
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Supersedes [DS93]. New V* without GCVS designation: the authors introduce a number after the constellation name. For those objects with only the constellation name (the authors say 'strictly provisional designation'), objects are in SIMBAD with an other designation when found. Since 2001, the catalogue is a 'living catalogue', see 2001PASP..113..764D, access via http://icarus.stsci.edu/~downes/cvcat/ .
Ref:	=1997PASP..109..345D
by	DOWNES R. , WEBBINK R.F., SHARA M.M.
	Publ. Astron. Soc. Pac., 109, 345-440 (1997)
	A catalog and atlas of cataclysmic variables-second edition.
o	Table 1: format 'CCC' not in SIMBAD, objects can be found via http://icarus.stsci.edu/~downes/cvcat/, in SIMBAD cross-id. in other columns are used. In ref list: Margon 1985PASP.97.962 instead of 912, SANFORD 1945PASP...57..312S instead of PASP.57.321, SHAFTER 1990ApJ...354..708 S instead of ApJ Lett, WEBBINK 1987ApJ...314..653W instead of ApJS.314
o	Table 1: <[DWS97] CCC N> N=143.
=E=	Catalogue in electronic form as V/110
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DWV2017]
[DWV2017]	(Dai+Wang+Vadakkumthani+, 2017)= ([DWV2017a])
Write:	<<[DWV2017] JHHMM.m XN>>
N:	24
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	N=26 X-ray sources in the field of ten 3FGL gamma-ray millisecond pulsars (MSPs). Use of archival X-ray observations from the Swift, Chandra, XMM-Newton, and Suzaku satellites.
Ref:	=2017RAA....17...72D
by	DAI X.-J. , WANG Z.-X., VADAKKUMTHANI J., XING Y.
	RAA, 17, 72 (2017)
	Identification of candidate millisecond pulsars from Fermi LAT observations II.
o	Table 4: <[DWV2017] JHHMM.m XN> N=24.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DWV2017a]
[DWV2017a]	(Dai+Wang+Vadakkumthani+, 2017)
*****	Avoid the usage of [DWV2017a], prefer [DWV2017]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DWV2017b]
[DWV2017b]	(Decarli+Walter+Venemans+, 2017)
Write:	<<[DWV2017b] SDSS J0842+1218 companion>> <<[DWV2017b] CFHQ J2100-1715 companion>> <<[DWV2017b] PSO JDDD+DD companion>>
N:	1+1+2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ALMA band 6 observations of N=4 galaxies at z>6 that are companions of quasars.
Ref:	=2017Natur.545..457D
by	DECARLI R. , WALTER F., VENEMANS B.P., BANADOS E., BERTOLDI F., CARILLI C., FAN X., FARINA E.P., MAZZUCCHELLI C., RIECHERS D., RIX H.-W., STRAUSS M.A., WANG R., YANG Y.
	Natur, 545, 457-461 (2017)
	Rapidly star-forming galaxies adjacent to quasars at redshifts exceeding 6.
o	Fig. 1, Table 1: <[DWV2017b] SDSS J0842+1218 companion> N=1, <[DWV2017b] CFHQ J2100-1715 companion> N=1, <[DWV2017b] PSO JDDD+DD companion> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DWV96]
[DWV96]	(Dougherty+Williams+Van der Hucht+, 1996)
Write:	<<[DWV96] WR 146 W>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=2 sources in WR 146, a bright northern source and a weaker southern one.
in source:	WR 146
Ref:	=1996MNRAS.280..963D
by	DOUGHERTY S.M. , WILLIAMS P.M., VAN DER HUCHT K.A., BODE M.F., DAVIS R.J.
	Mon. Not. R. Astron. Soc., 280, 963-970 (1996)
	Multifrequency observations of the Wolf-Rayet star WR 146 : another colliding-wind binary?
o	Table 1: <[DWV96] WR 146 N>, <[DWV96] WR 146 S>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DXJ2009]
[DXJ2009]	(Domingue+Xu+Jarrett+, 2009)
Write:	<<[DXJ2009] DDD.dddd+DD.dddd>>
N:	22
Object:	G in Pair + G (SIMBAD class: Galaxy)
Note:	KPNO 2.1m spectroscopic observations of galaxy pairs.
Ref:	=2009ApJ...695.1559D
by	DOMINGUE D.L. , XU C.K., JARRETT T.H., CHENG Y.
	Astrophys. J., 695, 1559-1566 (2009)
	2MASS/SDSS close major-merger galaxy pairs.
o	Table 1: <[DXJ2009] DDD.dddd+DD.dddd> N=22.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DXS
DXS	(Deep Extragalactic Survey)
*****	Avoid the usage of DXS, prefer [SES2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [DY2008]
[DY2008]	(Du+Yang, 2008)
Write:	<<[DY2008] NNa>> <<[DY2008] GLLL.ll+BB.bb>>
N:	61+39
Object:	IRDC (SIMBAD class: DarkNeb = Dark Cloud (nebula))
Note:	Purple Mountain Observatory 13.7m radio telescope CO line observations of infrared dark clouds. See also MSXDC.
Ref:	=2008ApJ...686..384D
by	DU F. , YANG J.
	Astrophys. J., 686, 384-398 (2008)
	A ^{12}CO, ^{13}CO, and C^{18}O survey of infrared dark clouds.
o	Table 1, col(1): <[DY2008] NN> (Nos 1-61) = Table 1, col(2): <[DY2008] GLLL.ll+BB.bb> N=61. Table 3: <[DY2008] NNa> N=39 added.
=E=	Catalogue in electronic form as <J/ApJ/686/384/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DYC2005]
[DYC2005]	(Drosdovsky+Yan+Chen+, 2005)
Write:	<<[DYC2005] NNN>>
N:	601
Object:	G (SIMBAD class: EmObj = Emission Object)
Note:	First results from the HST ACS Grism Parallel Survey.
Ref:	=2005AJ....130.1324D
by	DROZDOVSKY I. , YAN L., CHEN H.-W., STERN D., KENNICUTT R.Jr, SPINRAD H., DAWSON S.
	Astron. J., 130, 1324-1336 (2005)
	The Hubble Space Telescope ACS grism parallel survey. II. First results and a catalog of faint emission-line galaxies at z≤1.6.
o	Table 2: <[DYC2005] NNN> (Nos 1-601).
=E=	Catalogue in electronic form as J/AJ/130/1324
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DYH2009]
[DYH2009]	(Dasyra+Yan+Helou+, 2009)
Write:	<<[DYH2009] MIPS NNNNN>>
N:	150
Object:	IR-luminous G (SIMBAD class: Galaxy)
Note:	Spitzer IRS observations of N=150 infrared luminous galaxies in the Spitzer Extragalactic First Look Survey.
Ref:	=2009ApJ...701.1123D
by	DASYRA K.M. , YAN L., HELOU G., SAJINA A., FADDA D., ZAMOJSKI M., ARMUS L., DRAINE B., FRAYER D.
	Astrophys. J., 701, 1123-1146 (2009)
	The ~0.9 mJy sample: a mid-infrared spectroscopic catalog of 150 infrared-luminous, 24 µm selected galaxies at 0.3 ≤ z ≤ 3.5.
o	Table 1: <[DYH2009] MIPS NNNNN> N=150 among (Nos 34-22744).
=E=	Catalogue in electronic form as <J/ApJ/701/1123/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DYM92]
[DYM92]	(Dobashi+Yonekura+Mizuno+, 1992)
Write:	<<[DYM92] Cloud A>> <<[DYM92] Clump AN>> <<[DYM92] NN>>
N:	5+15+16
Object:	Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	Study of IC 5146 cloud complex: N=5 13CO clouds (Nos A-E).. N=15 Clumps in the clouds, format AN. N=16 IRAS sources cross-identified with a 'NN' numbering.
Ref:	=1992AJ....104.1525D
by	DOBASHI K. , YONEKURA Y., MIZUNO A., FUKUI Y.
	Astron. J., 104, 1525-1532 (1992)
	CO12 and CO13 observations of the dark cloud complex near IC 5146.
o	Fig.4, Table 1: <[DYM92] Cloud A> (Nos A-E). Fig.5, Table 1: <[DYM92] Clump AN> (Nos A1-A2, B1-B5, C1-C4, D1, E1-E3). Table 4: <[DYM92] NN> (Nos 1-16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DYZ2015]
[DYZ2015]	(Decker French+Yang+Zabludoff+, 2015)
Write:	<<[DYZ2015] EAANN>>
N:	32
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	IRAM 30m telescope EMIR 12CO(1-0) and 12CO(2-1) and SMT 10m telescope 12CO(2-10) observations of N=32 post-starburst galaxies. Use of archival SDSS DR7 data.
Ref:	=2015ApJ...801....1D
by	DECKER FRENCH K. , YANG Y., ZABLUDOFF A., NARAYANAN D., SHIRLEY Y., WALTER F., SMITH J.-D., TREMONTI C.A.
	Astrophys. J., 801, 1 (2015)
	Discovery of large molecular gas reservoirs in post-starburst galaxies.
o	Table 1: <[DYZ2015] EAHNN> (Nos 1-17), <[DYZ2015] EASNN> (Nos 1-15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DZ2013]
[DZ2013]	(Di Tullio Zinn+Zinn, 2013)
Write:	<<[DZ2013] SDSSNN>> <<[DZ2013] CNN>>
N:	18+75
Object:	GlCl + Poss. GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Note:	N=18 clusters and N=75 candidate clusters identified in the SDSS, searched for outer halo globular clusters around M31.
in source:	M 31 = NGC 224
Ref:	=2013AJ....145...50D
by	DI TULLIO ZINN G. , ZINN R.
	Astron. J., 145, 50 (2013)
	More remote globular clusters in the outer halo of M31.
o	Table 1: <[DZ2013] SDSSNN> (Nos SDSS1-SDSS18). Table 2: <[DZ2013] CNN> (Nos C1-C75).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DZ2014]
[DZ2014]	(Di Tullio Zinn+Zinn, 2014)
Write:	<<[DZ2014] A>>
N:	7
Object:	GlCl + Poss. GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Note:	Use of SDSS DR8 data to find N=6 globular clusters and N=1 likely candidate around M31 and M33 II.
Ref:	=2014AJ....147...90D
by	DI TULLIO ZINN G. , ZINN R.
	Astron. J., 147, 90 (2014)
	A search for globular clusters in more remote areas around M31 and M33 II.
o	Fig. 6, Tables 1-2: <[DZ2014] A> (Nos A-G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DZ2015]
[DZ2015]	(Di Tullio Zinn+Zinn, 2015)= (dTZZ) = ([DZ2015a])
Write:	<<[DZ2015] NN>> <<[DZ2015] CNN>> <<[DZ2015] M81-CN>>
N:	22+12+5
Object:	GlCl + Poss. GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	N=22 globular clusters and N=12 globular cluster candidates in M31 and also N=5 globular cluster candidates in the M81 Group, found in the SDSS. See also [DZ2013] and [DZ2014].
in source:	M 31 = NGC 224
in source:	NAME M 81 GROUP
Ref:	=2015AJ....149..139D
by	DI TULLIO ZINN G. , ZINN R.
	Astron. J., 149, 139 (2015)
	A search for intergalactic globular clusters in the Local Group.
o	Tables 1-2: <[DZ2015] NN> (Nos 1-22). Table 3: <[DZ2015] CNN> (Nos C01-C12). Table 4: <[DZ2015] M81-CN> (Nos C1-C5).
o	Objects in Figure 1 are not in Simbad.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DZ2015a]
[DZ2015a]	(Di Tullio Zinn+Zinn, 2015)= (dTZZ)
*****	Avoid the usage of [DZ2015a], prefer [DZ2015]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DZ2015b]
[DZ2015b]	(Diaz-Gimenez+Zandivarez, 2015)
Write:	<<[DZ2015b] NNN>>
N:	813
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=813 galaxy groups in the local Universe Use of 2MASX data.
Ref:	=2015A&A...578A..61D
by	DIAZ-GIMENEZ E. , ZANDIVAREZ A.
	Astron. Astrophys., 578A, 61-61 (2015)
	Where are compact groups in the local Universe?
o	Table B1: <[DZ2015b] NNN> N=813.
=E=	Catalogue in electronic form as J/A+A/578/A61
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DZA2012]
[DZA2012]	(Deharveng+Zavagno+Anderson+, 2012)
Write:	<<[DZA2012] BRCNN aN>> <<[DZA2012] BRCNN N>> <<[DZA2012] Sh201 aN>> <<[DZA2012] Sh201 N>> <<[DZA2012] IB aN>> <<[DZA2012] IB N>> <<[DZA2012] IB exN>> <<[DZA2012] Isolated NN>> <<[DZA2012] Isolated 14bis>>
N:	13+5+19+13+20+15 (SIMBAD class: Infrared = Infra-Red Source)
Note:	Herschel observations of W 5 EAST. Use of archival Spitzer and 2MASS photometry.
in source:	W 5e
Ref:	=2012A&A...546A..74D
by	DEHARVENG L. , ZAVAGNO A., ANDERSON L.D., MOTTE F., ABERGEL A., ANDRE P., BONTEMPS S., LELEU G., ROUSSEL H., RUSSEIL D.
	Astron. Astrophys., 546A, 74-74 (2012)
	Interstellar matter and star formation in W5-E. A Herschel view.
o	Tables 2,3,5,6,A.1,B.1,B.2,C.1,C.2,D.1 : <[DZA2012] BRCNN aN>,<[DZA2012] BRCNN N>,<[DZA2012] Sh201 aN>,<[DZA2012] Sh201 N>,<[DZA2012] IB aN>,<[DZA2012] IB N>,<[DZA2012] IB exN>,<[DZA2012] Isolated NN>,<[DZA2012] Isolated 14bis> N=13+5+19+13+20+15
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DZC2005]
[DZC2005]	(Deharveng+Zavagno+Caplan, 2005)
Write:	<<[DZC2005] A>>
N:	3
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	The authors found MSX point sources associated with the HII galactic regions: 3 new regions are found (Nos X, Y, Z), which are associated to NVSS radio sources. Among the sources given by the authors, two are not in the MSX point source catalogue.
Ref:	=2005A&A...433..565D
by	DEHARVENG L. , ZAVAGNO A., CAPLAN J.
	Astron. Astrophys., 433, 565-577 (2005)
	Triggered massive-star formation on the borders of Galactic HII regions. I. A search for ``collect and collapse'' candidates.
o	A C Fig.18: "the numbers of the sources in their Fig. 18 are reversed by mistake." (cf 2009A&A...494..987P)
o	Table 1: <[DZC2005] A> (Nos X, Y, Z).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DZC97]
[DZC97]	(Deharveng+Zavagno+Cruz-Gonzalez+, 1997)
Write:	<<[DZC97] NN>>
N:	55
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	NAME AFGL 4029 Cluster
Ref:	=1997A&A...317..459D
by	DEHARVENG L. , ZAVAGNO A., CRUZ-GONZALEZ I., SALAS L., CAPLAN J., CARRASCO L.
	Astron. Astrophys., 317, 459-475 (1997)
	AFGL 4029: a cluster of massive young stars.
o	Table 2: IRS 1, 2 = [TTH80] IRS 1, 2
o	<NAME AFGL 4029 CLUSTER>. Table 1: <[DZC97] NN> (Nos 1-55)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DZD2003]
[DZD2003]	(De Rijcke+Zeilinger+Dejonghe+, 2003) (Not yet in Simbad)
Write:	<<[DZD2003] CLN>>
N:	6
Object:	Cloud (SIMBAD class: Cloud)
Note:	N=6 faint HII emission cloud in FCC 46.
in source:	FCC 46
Ref:	=2003MNRAS.339..225D
by	DE RIJCKE S. , ZEILINGER W.W., DEJONGHE H., HAU G.K.T.
	Mon. Not. R. Astron. Soc., 339, 225-234 (2003)
	Evidence for a warm interstellar medium in the Fornax dwarf ellipticals FCC046 and FCC207.
o	Table 1, Fig.9: <[DZD2003] CLN> (Nos CL1-CL6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DZN99]
[DZN99]	(Deharveng+Zavagno+Nadeau+, 1999)
Write:	<<[DZN99] NNN>>
N:	424
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	SH 2-138
Ref:	=1999A&A...344..943D
by	DEHARVENG L. , ZAVAGNO A., NADEAU D., CAPLAN J., PETIT M.
	Astron. Astrophys., 344, 943-954 (1999)
	Sh 138: a compact HII region excited by a very young cluster.
o	Table 1: <[DZN99] NNN> (Nos 1-424).
=E=	Catalogue in electronic form as J/A+A/344/943
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: DZOA
DZOA	(DENIS ZoA)
Write:	<<DZOA NNNN-NN>>
N:	153
Object:	G (SIMBAD class: Galaxy)
Note:	Search for galaxies around PKS 1343-601 on images of the NIR DENIS survey.
Ref:	=2007A&A...466..481S
by	SCHROEDER A.C. , MAMON G.A., KRAAN-KORTEWEG R.C., WOUDT P.A.
	Astron. Astrophys., 466, 481-499 (2007)
	The highly obscured region around PKS 1343-601. I. Galactic interstellar extinctions using DENIS galaxy colours.
o	Tables 2, 3: <DZOA NNNN-NN> N=126+27.
=E=	Catalogue in electronic form as J/A+A/466/481
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DZP97]
[DZP97]	(De ruiter+Zamorani+Parma+, 1997)
Write:	<<[DZP97] NNNa>>
N:	160
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
in source:	NAME Lockman Hole
Ref:	=1997A&A...319....7D
by	DE RUITER H.R. , ZAMORANI G., PARMA P., HASINGER G., HARTNER G., TRUEMPER J., BURG R., GIACCONI R., SCHMIDT M.
	Astron. Astrophys., 319, 7-17 (1997)
	Deep radio observations of the "Lockman Hole".
o	Tables 2, 3, col(1): RDS NN or NNA in SIMBAD.
o	Table 1: <[DZP97] NNNa> (Nos 1-149) N=160
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DZR2017]
[DZR2017]	(Dessauges-Zavadsky+Zamojski+Rujopakarn+, 2017)
Write:	<<[DZR2017] MACS J0032-arc>> <<[DZR2017] MACS J0032-arc A>>
N:	1+6
Object:	Grav. lensed image of a G (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy)
Note:	IRAM PdBI observations, and NRAO JVLA observations of N=1+6 gravitationally lensed images of a galaxy, lensed by the galaxy cluster MCS J0032.1+1808. Use of HST ACS, Spitzer IRAC, and Herschel SPIRE data.
in source:	MCS J0032.1+1808
Ref:	=2017A&A...605A..81D
by	DESSAUGES-ZAVADSKY M. , ZAMOJSKI M., RUJOPAKARN W., RICHARD J., SKLIAS P., SCHAERER D., COMBES F., EBELING H., RAWLE T.D., EGAMI E., BOONE F., CLEMENT B., KNEIB J.-P., NYLAND K., WALTH G.
	Astron. Astrophys., 605A, 81-81 (2017)
	Molecular gas properties of a lensed star-forming galaxy at z ~ 3.6: a case study.
o	<[DZR2017] MACSJ0032-arc> N=1. Fig. 1, Table 1: <[DZR2017] MACSJ0032-arc A> (Nos A-F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DZS2003]
[DZS2003]	(Deharveng+Zavagno+Salas+, 2003) (Not yet in Simbad)
Write:	<<[DZS2003] Sh 219 NNN>> <<[DZS2003] Sh 217 NNN>>
N:	221+124
Object:	* (SIMBAD class: Star)
Note:	Stars in fields centered on the HII regions Sh 2-219 and Sh 2-217.
in source:	SH 2-219
in source:	SH 2-217
Ref:	=2003A&A...399.1135D
by	DEHARVENG L. , ZAVAGNO A., SALAS L., PORRAS A., CAPLAN J., CRUZ-GONZALEZ I.
	Astron. Astrophys., 399, 1135-1145 (2003)
	Sequential star formation at the periphery of the HII regions Sh 217 and Sh 219.
o	Table 3: <[DZS2003] Sh 219 NNN> N=221 among (Nos 1-223). Table 4: <[DZS2003] Sh 217 NNN> (Nos 1-124).
=E=	Catalogue in electronic form as J/A+A/199/1135
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DZS2003]
[DZS2003]	(Deharveng+Zavagno+Salas+, 2003)
Write:	<<[DZS2003] Sh 219 NNN>> <<[DZS2003] Sh 217 NNN>>
N:	221+124
Object:	* (SIMBAD class: Star)
Note:	Stars in 2 fields centered on 2 HII regions Sh 2-219 and Sh 2-217.
Ref:	=2003A&A...399.1135D
by	DEHARVENG L. , ZAVAGNO A., SALAS L., PORRAS A., CAPLAN J., CRUZ-GONZALEZ I.
	Astron. Astrophys., 399, 1135-1145 (2003)
	Sequential star formation at the periphery of the HII regions Sh 217 and Sh 219.
o	Table 3: <[DZS2003] Sh 219 NNN> N=221 among (Nos 1-223). Table 4: <[DZS2003] Sh 217 NNN> (Nos 1-124).
=E=	Catalogue in electronic form as J/A+A/399/1135
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DZS2009]
[DZS2009]	(Deharveng+Zavagno+Schuller+, 2009)
Write:	<<[DZS2009] NNN>> <<[DZS2009] Condensation N>> <<[DZS2009] Condensation N core>> <<[DZS2009] Condensation N bis>> <<[DZS2009] Condensation N aN>>
N:	139+19
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	APEX LABOCA 870mum and Spitzer/MIPS 24mum and 70mum observations of RCW 120. See also <[ZPD2007]>.
in source:	RCW 120
Ref:	=2009A&A...496..177D
by	DEHARVENG L. , ZAVAGNO A., SCHULLER F., CAPLAN J., POMARES M., DE BREUCK C.
	Astron. Astrophys., 496, 177-190 (2009)
	Star formation around RCW 120, the perfect bubble.
o	Table 1: <[DZS2009] NNN> (Nos 1-138). Table 2: <[DZS2009] Condensation N> (Nos 1-9), <[DZS2009] Condensation 1 core>, <[DZS2009] Condensation 2 bis>, <[DZS2009] Condensation N aN> N=-. Table 2: <[ZPD2007] CN> (No. 9) added.
Ref:	=2010A&A...518L..81Z
by	ZAVAGNO A. , RUSSEIL D., MOTTE F., ANDERSON L.D., DEHARVENG L., RODON J.A., BONTEMPS S., ABERGEL A., BALUTEAU J.-P., SAUVAGE M., ANDRE P., HILL T., WHITE G.J.
	Astron. Astrophys., 518L, 81-81 (2010)
	Star formation triggered by the galactic HII region RCW 120. First results from the Herschel Space Observatory.
o	Table 1: <[DZS2009] NNN> (No. 0 added).
=E=	Catalogue in electronic form as J/A+A/496/177
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [DZS2015]
[DZS2015]	(Deharveng+Zavagno+Samal+, 2015)
Write:	<<[DZS2015] 2-CN>> <<[DZS2015] 4-CN>>
N:	3+7
Object:	smm Clump (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	Herschel Hi-GAL and MALT90 observations of N=3+7 dense molecular clumps in N=2 bipolar HII regions G319.88+00.79 and G010.32-00.15. Use of 870µm data from the APEX ATLASGAL survey of the Galactic plane. Use of archival Herschel SPIRE data. See also [BLH2011] and [WWS2012].
in source:	GAL 319.88+00.79
in source:	GAL 010.30-00.15
Ref:	=2015A&A...582A...1D
by	DEHARVENG L. , ZAVAGNO A., SAMAL M.R., ANDERSON L.D., LELEU G., BREVOT D., DUARTE-CABRAL A., MOLINARI S., PESTALOZZI M., FOSTER J.B., RATHBORNE J.M., JACKSON J.M.
	Astron. Astrophys., 582A, 1-1 (2015)
	Bipolar HII regions - Morphology and star formation in their vicinity. I. G319.88+00.79 and G010.32-00.15.
o	Table 2: <[DZS2015] 2-CN> (Nos C1-C3). Table 4: <[DZS2015] 4-CN> (Nos C1-C7)>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: E
E	(Edinburgh obs.) (Not yet in Simbad)
*****	Avoid the usage of E, prefer Edinburgh
Origin	of the Acronym: L = Found in the literature
Details on Acronym: E
E	(Edinburgh obs.)
*****	Avoid the usage of E, prefer Bruck
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: E
E	(E region)
*****	Avoid the usage of E, prefer [CS62]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: E
E	(Einstein obs.)
====>	Equivalent to: 1E
Details on Acronym: E
E	(Ebbighausen)
*****	Avoid the usage of E, prefer [E38]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: E
E	(Einstein Obs.)
*****	Avoid the usage of E, prefer [FT84]
Origin	of the Acronym: L (1999A&A...342..101V)
Details on Acronym: E
E	(Sgr E)
*****	Avoid the usage of E, prefer [GWC93]
Origin	of the Acronym: L (1996MNRAS.280.1110C)
Details on Acronym: E
E	(ESO (B) plates)
Write:	<<NAME E N>>
N:	3
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Note:	N=3 probable GCl. E1 = AM-1 = ESO 201-10, galactocentric distance 118 kpc (Aaronson+, 1984ApJ...276..221A and plates 1 and 2). E2 = ESO 120-8. E3 = ESO 37-1
Ref:	=1976A&A....52..309L
by	LAUBERTS A.
	Astron. Astrophys., 52, 309-311 (1976)
	Three distant stellar clusters found on ESO blue survey plates.
o	Table 1: <NAME EN> (Nos E1 to E3)
Details on Acronym: E
E	(E region)
Write:	<<NAME E N REGION>>
N:	9
Object:	Region (SIMBAD class: Region = Region defined in the Sky)
Note:	See also stars in each region: [CS62].
Ref:	=1962RGOB...49....3C
by	COUSINS A.W.J. , STOY R.H.
	R. Obs. Bull., 49, 3-None (1962)
	Standard magnitudes in the E regions.
o	<[CS62] EN NNN> N=801, <[CS62] EN A> N=3, <[CS62] EN a> N=60. <NAME E1 REGION> to <NAME E9 REGION> N=9
=E=	Catalogue in electronic form as II/222
Details on Acronym: E
E	(Early-type star)
*****	Avoid the usage of E, prefer [PGM2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: E
E	(Einstein obs.)
*****	Avoid the usage of E, prefer TF
Origin	of the Acronym: L = Found in the literature
Details on Acronym: E-CDF-S
E-CDF-S	(Extended-CDFS)
*****	Avoid the usage of E-CDF-S, prefer [LBA2005]
Origin	of the Acronym: L (2006AJ....131.2826S)
Details on Acronym: 1E
1E	(Einstein obs., 1st version)= E = EMSS = (IE) = (MS)
Write:	<<1E HHMM+DD.d>> <<1E HHMM.m+DDMM>> <<1E HHMMSS+DDMM.m>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat.	in SIMBAD: for EMSS only
Note:	EMSS objects are designated 1E in SIMBAD (Optical identif. in ref. 1991ApJS...76..813S, Atlas in ref. 1994ApL....29..267M). See also [LSE2002].
Ref:	=1981ApJ...245..163V
by	VAIANA G.S. , CASSINELLI J.P., FABBIANO G., GIACCONI R., GOLUB L., GORENSTEIN P., HAISCH B.M., HARNDEN F.R., JOHNSON H.M., LINSKY J.L., MAXSON C.W., MEWE R., ROSNER R., SEWARD F., TOPKA K., ZWAAN C.
	Astrophys. J., 245, 163-182 (1981)
	Results from an extensive Einstein stellar survey.
o	Table 1: <1E HHMM.m+DDMM>, <1E HHMMSS+=DDMM.m>, N=144
Ref:	=1982ApJ...253..504M
by	MACCACARO T. , FEIGELSON E.D., FENER M., GIACCONI R., GIOIA I.M., GRIFFITHS R.E., MURRAY S.S., ZAMORANI G.
	Astrophys. J., 253, 504-511 (1982)
	A medium sensitivity X-ray survey using the Einstein Observatory: the log N-log S relation for extragalactic X-ray sources.
o	Table 1: <1E HHMM.m+DDMM> N=63
Ref:	=1984ApJ...283..495G
by	GIOIA I.M. , MACCACARO T., SCHILD R.E., STOCKE J.T., LIEBERT J.W., DANZIGER I.J., KUNTH D., LUB J.
	Astrophys. J., 283, 495-511 (1984)
	The medium sensivity survey: a new sample of X-ray sources with optical identifications and the revised extragalactic log N-log S.
o	Table 2: <1E HHMM.m+DDMM> N=50, 49 are new.
Ref:	=1984ApJ...278..137H
by	HERTZ P. , GRINDLAY J.E.
	Astrophys. J., 278, 137-149 (1984)
	The Einstein galactic plane survey : statistical analysis of the complete X-ray sample.
o	Table 3: <1E HHMM.m+DDMM> N=71
Ref:	=1988AJ.....96..233H
by	HERTZ P. , GRINDLAY J.E.
	Astron. J., 96, 233-241 (1988)
	The Einstein galactic plane survey. II. Optical observations of northern hemisphere X-ray sources.
o	Table II: stars in error boxes, format 'A', are not in SIMBAD
o	Table I: <1E HHMM.m+DDMM> N=67
Ref:	=1990ApJS...72..567G
by	GIOIA M. , MACCACARO T., SCHILD R.E., WOLTER A., STOCKE J.T., MORRIS S.L., HENRY J.P.
	Astrophys. J., Suppl. Ser., 72, 567-619 (1990)
	The Einstein Observatory extended medium-sensitivity survey. I. X-ray data and analysis.
o	Table 3: EMSS use <1E HHMM.m+DDMM> N=835
Ref:	=1991ApJS...76..813S
by	STOCKE J.T. , MORRIS S.L., GIOIA I.M., MACCACARO T., SCHILD R., WOLTER A., FLEMING T.A., HENRY J.P.
	Astrophys. J., Suppl. Ser., 76, 813-874 (1991)
	The Einstein Observatory extended medium-sensitivity survey. II. The optical identifications.
o	EMSS use <1E HHMM.m+DDMM>
Ref:	=1994ApL....29..267M
by	MACCACARO T. , WOLTER A., McLEAN B., GIOIA I.M., STOCKE J.T., DELLA CECA R., BURG R., FACCINI R.
	Astrophys. Lett., 29, 267-272 (1994)
	The Einstein observatory extended medium sensitivity survey. III. The atlas of optical finding charts.
o	EMSS use <1E HHMM.m+DDMM>
=E=	Catalogue in electronic form as IX/15
Details on Acronym: 2E
2E	(Einstein obs., 2nd version)= (IPC)
Write:	<<2E HHMM.m+DDMM>> <<2E NNNN>>
N:	9612
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Ref:	=1994HEAO2.C......0M
by	McDOWELL J.C.
	Einstein Obs. Unscreened IPC Data Archive, 0-None (1994)
	The Einstein Observatory Soft X-ray Source List.
o	SAO HEAD CD-ROM Series I (Einstein), Nos 18-36
o	<2E HHMM.m+DDMM>, <2E NNNN>, <0ES HHMM+DD.d>.
=E=	Catalogue in electronic form as IX/13
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [E2000]
[E2000]	(Eisloffel, 2000) (Not yet in Simbad)
Write:	<<[E2000] NGC 2071 R>> <<[E2000] NGC 2071 R A>> <<[E2000] NGC 7129 R>> <<[E2000] NGC 7129 R A>>
N:	12+9+10+2
Object:	Molecular Outflow (SIMBAD class: PartofCloud = Part of Cloud)
Note:	Format 'R': Molecular outflows, (Nos I-XII) in NGC 2071, (Nos I-IX) in NGC 7129. Format 'R A': knotty jets in the outflows.
in source:	NGC 2071
in source:	NGC 7129
Ref:	=2000A&A...354..236E
by	EISLOEFFEL J.
	Astron. Astrophys., 354, 236-246 (2000)
	Parsec-scale molecular H_{2} outflows from young stars.
o	Figs 1, 2: <[DDM94] Knot A> (Nos M-S) added. Fig.3: <[E2000] NGC 2071 R> (Nos I-XII), <[E2000] NGC 2071 R A> N=10. Fig.5: <[E2000] NGC 7129 R> (Nos I-IX), <[E2000] NGC 7129 R A> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [E2005]
[E2005]	(Ellingsen, 2005) (Not yet in Simbad)
Write:	<<[E2005] LLL.ll+B.bb>> <<[E2005] LLL.lll+B.bbb>>
N:	86
Object:	CH3OH Maser (SIMBAD class: Maser)
Note:	Australia Telescope National Facility Mopra mm telescope is used to search for methanol masers. See also [EVM96], Caswell.
Ref:	=2005MNRAS.359.1498E
by	ELLINGSEN S.P.
	Mon. Not. R. Astron. Soc., 359, 1498-1516 (2005)
	The relationship between class I and class II methanol masers.
o	Table 5: <[E2005] LLL.ll+B.bb>, <[E2005] LLL.lll+B.bbb>, N=86.
=E=	Catalogue in electronic form as J/MNRAS/359/1498
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [E2007]
[E2007]	(Ellingsen, 2007) (Not yet in Simbad)
Write:	<<[E2007] GLLL.ll+B.bb>>
N:	38
Object:	CH3OH Maser (SIMBAD class: Maser)
Note:	Search for methanol masers towards GPSC sources. See also [PMB2005], [SKH2002].
Ref:	=2007MNRAS.377..571E
by	ELLINGSEN S.P.
	Mon. Not. R. Astron. Soc., 377, 571-583 (2007)
	A GLIMPSE-based search for 6.7-GHz methanol masers and the lifetime of their spectral features.
o	Table 1: <[E2007] GLLL.ll+B.bb> N=38.
=E=	Catalogue in electronic form as J/MNRAS/377/571
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [E2009]
[E2009]	(El Bouchefry, 2009)
Write:	<<[E2009] NN>>
N:	79
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Sample of N=79 radio-emitting X-ray sources in the XBootes field, using data from the FIRST, NDWFS, and Chandra XBootes surveys.
Ref:	=2009MNRAS.396.2011E
by	EL BOUCHEFRY K.
	Mon. Not. R. Astron. Soc., 396, 2011-2037 (2009)
	X-ray identifications of FIRST radio sources in the XBootes field.
o	Table 1: <[E2009] NN> (Nos 1-79).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [E38]
[E38]	(Ebbighausen, 1938)= (E)
Write:	<<[E38] NN>>
N:	99
Object:	PM* (SIMBAD class: HighPM* = High Proper Motion Star)
Note:	The list is not numbered by the author, but found numbered in the literature. Numerous cross-id. with BD No.
Ref:	=1938AJ.....47..112E
by	EBBIGHAUSEN E.G.
	Astron. J., 47, 112-113 (1938)
	A list of 99 proper motion stars.
o	<[E38] NN> (Nos 1-99), list not numbered here, but found numbered in literature
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [E61]
[E61]	(Eggen, 1961) (Not yet in Simbad)
Write:	<<[E61] NN>>
N:	11
Object:	* (SIMBAD class: Star)
Note:	N=11 secondary standards in a LMC field.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1961RGOB...27...61E
by	EGGEN O.J.
	R. Obs. Bull., 27, 61-None (1961)
	Three-colour photometry in the southern hemisphere NGC 6383, NGC 6405 and standard stars.
o	Table I: <Cl* NGC 3114 E A> (Nos X, Y). Table II, Plate 1: <[E61] NN> (Nos 1-11). Table III: <NGC 6383 NN> (Nos 1-25). Table IV: <Cl* NGC 6405 E NNa> (Nos 31a-31e, 32a-32c, 54a, 66a).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [E73]
[E73]	(Ebisch, 1973)
Write:	<<[E73] NN>>
N:	26
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Ref:	=1973PASP...85..746E
by	EBISCH K.E.
	Publ. Astron. Soc. Pac., 85, 746-750 (1973)
	A distant cephei variable in Centaurus.
o	Tables I, II: <[E73] NN> (Nos 1-26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [E75]
[E75]	(Eggen, 1975)
Write:	<<[E75] N>>
N:	6
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=6 stars near HR 5999-HR 6000. Nos 4 and 6 are variable.
Ref:	=1975PASP...87...37E
by	EGGEN O.J.
	Publ. Astron. Soc. Pac., 87, 37-63 (1975)
	Structure and age of the local association (Pleiades group).
o	Table IX: <[E75] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [E83]
[E83]	(Erickson, 1983)
Write:	<<[E83] 4C 21.53W>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	4C 21.53 is composed of at least 2 sources, named E ast and West by the authors.
in source:	4C 21.53
Ref:	=1983ApJ...264L..13E
by	ERICKSON W.C.
	Astrophys. J., 264, 13-17 (1983)
	What is 4C 21.53 ?
o	<[E83] 4C 21.53W> (Nos E, W).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [E85]
[E85]	(Eales, 1985)
Write:	<<[E85] HHMMSS+DDMMSS>> <<[E85] A>>
N:	1+8
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	CCD imaging observations of a newly discovered cluster of galaxies: '104603+354728' associated with the source 6C 1045+3547. Plate 1: in the field (Nos A-D) are possible optical identifications of the 6C source, (Nos E-H) are the brightest galaxies in the field.
Ref:	=1985MNRAS.214...27E
by	EALES S.A.
	Mon. Not. R. Astron. Soc., 214, 27-32 (1985)
	CCD observations of a rich distant cluster of galaxies (1046+35) containing a classical double radio source.
o	ClG 1046+35 = [E85] 104603+354728.
o	Text: <[E85] HHMMSS+DDMMSS> N=1. Table 1: <[E85] A> (Nos A-H).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [E85b]
[E85b]	(Eales, 1985)
Write:	<<[E85b] 1028+35 a>>
N:	10
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Search for possible optical identifications of 6C radio-sources. (Nos a-j) are galaxies in the field of B2 1028+35 = 6C 1028+3517.
Ref:	=1985MNRAS.217..167E
by	EALES S.A.
	Mon. Not. R. Astron. Soc., 217, 167-177 (1985)
	A sample of 6C sources selected at the peak of the source counts -II. Optical identifications.
o	Table 1: 1045+35C = 6C 1045+3547, 1045+35C a to d = [E85] A to D.
o	Table 1: <[E85b] 1028+35 a> (Nos a-j).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: E96
E96	(Eisenhardt+, 1996)
*****	Avoid the usage of E96, prefer [EAH96]
Origin	of the Acronym: L (1999AJ....117..671N)
Details on Acronym: EA
EA	(E+A)
*****	Avoid the usage of EA, prefer [ZZL96]
Origin	of the Acronym: L (2008ApJ...688..945Y)
Details on Acronym: [EAB95]
[EAB95]	(Elbaz+Arnaud+Bohringer, 1995)
Write:	<<[EAB95] ACO 2163 A>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations of ACO 2163. N=3 bright enhancements A to C.
in source:	ACO 2163
Ref:	=1995A&A...293..337E
by	ELBAZ D. , ARNAUD M., BOEHRINGER H.
	Astron. Astrophys., 293, 337-346 (1995)
	The gas distribution and binding mass in the A 2163 cluster.
o	Bright galaxies G1 and G2 in paragr. 5 are later designated as [MCF2008] BCG-1 and [MCF2008] BCG-2.
o	Text: <[EAB95] ACO 2163 A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EAC2018]
[EAC2018]	(Ercan+Aktekin+Cesur+, 2018)
Write:	<<[EAC2018] NN>>
N:	13
Object:	Poss. SNR (SIMBAD class: SNRemnant_Candidate = SuperNova Remnant Candidate)
Stat:	is completely incorporated in Simbad
Note:	TUBITAK 1.5m telescope RTT150 spectroscopic observations of N=13 SNR candidates in the galaxy NGC 1569.
in source:	NGC 1569
Ref:	=2018MNRAS.481.2804E
by	ERCAN E.N. , AKTEKIN E., CESUR N., TUMER A.
	Mon. Not. R. Astron. Soc., 481, 2804-2812 (2018)
	Optical and X-ray observational search for the possible supernova remnant candidates in the nearby galaxy NGC 1569.
o	Table 3: <[EAC2018] NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EAD
EAD	(Elias Accidental Detection)
Write:	<<EAD N>>
N:	2
Object:	G (SIMBAD class: RadioG = Radio Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLA 20cm observations. Serendipitous detection of 2 radio galaxies in ZwCl 1437+6436.
in source:	ZwCl 1437+6436
Ref:	=1991AJ....102...30E
by	ELIAS II N.M. , STRUBLE M.F.
	Astron. J., 102, 30-33 (1991)
	Discovery of two radio galaxies in the Zwicky cluster 1437.3+6436.
o	<EAD N> (Nos 1-2)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EAD2001]
[EAD2001]	(Ellis+Abraham+Dickinson, 2001)
Write:	<<[EAD2001] HDFN JHHMMSS.ss+DDMMSS.s>> <<[EAD2001] HDFS JHHMMSS.ss+DDMMSS.s>>
N:	255
Object:	G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Sample of early-type and spiral galaxies from HDFN and HDFS.
in source:	NAME HDFN
in source:	NAME HDFS
Ref:	=2001ApJ...551..111E
by	ELLIS R.S. , ABRAHAM R.G., DICKINSON M.
	Astrophys. J., 551, 111-130 (2001)
	The relative star formation histories of spiral bulges and elliptical galaxies in the Hubble deep fields.
o	Table 1: <[EAD2001] HDFN JHHMMSS.ss+DDMMSS.s>, <[EAD2001] HDFS JHHMMSS.ss+DDMMSS.s>, N=255.
=E=	Catalogue in electronic form as J/ApJ/551/111
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EAD2007]
[EAD2007]	(Estrada+Annis+Diehl+, 2007)
Write:	<<[EAD2007] SDSS +DDD.d+DD.d+z.zz>> <<[EAD2007] SDSS +DDD.ddd+DD.ddd+z.zz>> <<[EAD2007] Arc Na>>
N:	27+3+2
Object:	Cluster of G + Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	SDSS J014656.00-092952.5 cluster lens system: the giant Hall's Arc is divided in several arcs.
in source:	NAME Hall's Arc
Ref:	=2007ApJ...660.1176E
by	ESTRADA J. , ANNIS J., DIEHL H.T., HALL P.B., LAS T., LIN H., MAKLER M., MERRITT K.W., SCARPINE V., ALLAM S., TUCKER D.
	Astrophys. J., 660, 1176-1185 (2007)
	A systematic search for high surface brightness giant arcs in a Sloan Digital Sky Survey cluster sample.
o	Table 1 : SDSS have a format DDD.ddd+DD.d+z (RA and Dec in °.) which has been translated by the SIMBAD team into the correct designations. Ex : SDSS +239.6+27.2+0.11 = SDSS J155832.09+271050.9.
o	Tables 1-3: <[EAD2007] SDSS +DDD.ddd+DD.d+Z.zz> N=20+6+1. Tables 4, 5: <[EAD2007] Arc Na> (Nos 1-3, 1a-1b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EAH96]
[EAH96]	(Eisenhardt+Armus+Hogg+, 1996)= (E96)
Write:	<<[EAH96] Component N>>
N:	5
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=5 Components of the IRAS F10214+4724 lensed IR QSO.
in source:	IRAS F10214+4724
Ref:	=1996ApJ...461...72E
by	EISENHARDT P.R. , ARMUS L., HOGG D.W., SOIFER B.T., NEUGEBAUER G., WERNER M.W.
	Astrophys. J., 461, 72-83 (1996)
	Hubble Space Telescope observations of the luminous IRAS source FSC 10214+4724: a gravitationally lensed infrared quasar.
o	Star A and Star H = [RBL91] A and [RBL91] H.
o	Table 1: <[RBL91] A> (No. H) added. Table 1: <[EAH96] Component N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EAS91]
[EAS91]	(Ellis+Allington-Smith+Smail, 1991)
Write:	<<[EAS91] Arc WN>>
N:	2+6
Object:	Arc + Arclet (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Stat:	is completely incorporated in Simbad
Note:	WHT ISIS observations. Spectroscopic confirmation of giant arcs seen in ACO 963. The 2 arcs were first noted in 1988ApJ...329L..21L.
in source:	ACO 963
Ref:	=1991MNRAS.249..184E
by	ELLIS R. , ALLINGTON-SMITH J., SMAIL I.
	Mon. Not. R. Astron. Soc., 249, 184-190 (1991)
	Spectroscopy of arcs in the rich cluster Abell 963.
o	Fig.1, Table 1: <[EAS91] Arc W> (Nos N, S), <[EAS91] Arc WN> (Nos S1-S6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EB
EB	(Evans+Blair)= (IRS)
Write:	<<EB IRS NN>>
N:	12
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	SH 2-235
Ref:	=1981ApJ...246..394E
by	EVANS II N.J. , BLAIR G.N.
	Astrophys. J., 246, 394-408 (1981)
	The energetics of molecular clouds. III. The S235 molecular cloud.
o	Shells in T.6 not in Simbad
o	Table 5: <EB IRS NN> (Nos 1-12)
Origin	of the Acronym: L (1981ApJ...246..409E)
Details on Acronym: [EBB77]
[EBB77]	(Evans+Blair+Beckwith, 1977) (Not yet in Simbad)
Write:	<<[EBB77] N>>
N:	6
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
in source:	SH 2-255
Ref:	=1977ApJ...217..448E
by	EVANS II N.J. , BLAIR G.N., BECKWITH S.
	Astrophys. J., 217, 448-463 (1977)
	The energetics of molecular clouds. I. Methods of analysis and application to the S255 molecular cloud.
o	Table 4: <[EBB77] N> (Nos 1-6)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EBE2007]
[EBE2007]	(Eyles+Bunker+Ellis+, 2007)
Write:	<<[EBE2007] NN-NNNNN>>
N:	31
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	GOODS HST and Spitzer data are coupled with VLT ISAAC NIR observations to search for z about 6 galaxies.
Ref:	=2007MNRAS.374..910E
by	EYLES L.P. , BUNKER A.J., ELLIS R.S., LACY M., STANWAY E.R., STARK D.P., CHIU K.
	Mon. Not. R. Astron. Soc., 374, 910-930 (2007)
	The stellar mass density at z ~ 6 from Spitzer imaging of i'-drop galaxies.
o	Table 1: <[EBE2007] NN-NNNNN> N=31.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EBE82]
[EBE82]	(Elsasser+Birkle+Eiroa+, 1982)= (VES)
Write:	<<[EBE82] N>>
N:	2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	NGC 7538
Ref:	=1982A&A...108..274E
by	ELSAESSER H. , BIRKLE K., EIROA C., LENZEN R.
	Astron. Astrophys., 108, 274-278 (1982)
	On the infrared sources 1 and 2 in NGC 7538.
o	Table 1: VES use <[EBE82] N> (Nos 1-2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EBG2008]
[EBG2008]	(Eisenhardt+Brodwin+Gonzalez+, 2008)= (IRAC)
Write:	<<[EBG2008] IRAC JHHMMSS.s+DDMMSS>> <<[EBG2008] ser JHHMMSS.s+DDMMSS>>
N:	97+7
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC Shallow Survey. Search for galaxies in 12 ISCS clusters. Some serendipitous sources (ser in the format) are found.
Ref:	=2008ApJ...684..905E
by	EISENHARDT P.R.M. , BRODWIN M., GONZALEZ A.H., STANFORD S.A., STERN D., BARMBY P., BROWN M.J.I., DAWSON K., DEY A., DOI M., GALAMETZ A., JANNUZI B.T., KOCHANEK C.S., MEYERS J., MOROKUMA T., MOUSTAKAS L.A.
	Astrophys. J., 684, 905-932 (2008)
	Clusters of galaxies in the first half of the universe from the IRAC Shallow Survey.
o	Table 1: <ISCS JHHMM.m+DDMM> N=12. Table 3: <[EBG2008] IRAC JHHMMSS.s+DDMMSS> N=97, <[EBG2008] ser JHHMMSS.s+DDMMSS> N=7.
=E=	Catalogue in electronic form as <J/ApJ/684/905/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EBG2016]
[EBG2016]	(Eisner+Bally+Ginsburg+, 2016)
Write:	<<[EBG2016] GeMS NN>> <<[EBG2016] HCNNN>>
N:	40+33
Object:	* + (mm) (SIMBAD class: Star)
Note:	Gemini-S GeMS photometric and ALMA Cycle 6 observations of N=40 NIR stars and N=33 mm sources in the Orion Nebula cluster (ONC). See also [HC2000].
in source:	NAME ONC
Ref:	=2016ApJ...826...16E
by	EISNER J.A. , BALLY J.M., GINSBURG A., SHEEHAN P.D.
	Astrophys. J., 826, 16-16 (2016)
	Protoplanetary disks in the Orion OMC1 region imaged with ALMA.
o	Table 1: <[EBG2016] GeMS NN> (Nos 1-40). Table 3: <[EBG2016] HCNNN> N=33 among (Nos 779-819).
=E=	Catalogue in electronic form as <J/ApJ/826/16/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EBI2003]
[EBI2003]	(Eales+Bertoldi+Ivison+, 2003)= (MAMBO) (Not yet in Simbad)
Write:	<<[EBI2003] LH-MM NN>> <<[EBI2003] NTT-MM NN>> <<[EBI2003] A2125-MM NN>>
N:	2+21+11
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	MAMBO survey on the IRAM 30m telescope at 850mu.m in 3 fields: The Lockman Hole, The New Technology Telescope deep field (NTT), and a field centered on ACO 2125. For the NTT sources, see also [DLL2002], [DLL2004]. For the Lockman Hole sources, see also [GIB2004].
Ref:	=2003MNRAS.344..169E
by	EALES S. , BERTOLDI F., IVISON R., CARILLI C., DUNNE L., OWEN F.
	Mon. Not. R. Astron. Soc., 344, 169-180 (2003)
	SCUBA observations of the sources detected in the MAMBO 1200-µm survey.
o	Table 1: <[EBI2003] LH-MM NN> N=2 (Nos 13, 86), <[EBI2003] NTT-MM NN> N=8 among (Nos 1-34), <[EBI2003] A2125-MM NN> N=11 among (Nos 2-50).
Ref:	=2004ApJ...606..664D
by	DANNERBAUER H. , LEHNERT M.D., LUTZ D., TACCONI L., BERTOLDI F., CARILLI C., GENZEL R., MENTEN K.M.
	Astrophys. J., 606, 664-682 (2004)
	The faint counterparts of MAMBO millimeter sources near the New Technology Telescope Deep Field.
o	Introd. : SMM 02399-0314 is a misprint for SMM J02399-0134, Parag. 4 : LE 850.12 = [SFD2002] LHE 12
o	Table 1, col(1): <[DLL2002] MM JHHMMSS+DDMM.m> N=15 added. Table 1, col(2): <[EBI2003] NTT-MM NN> N=12 added among (Nos 7-42). Table 1, col(6,7): <DLL2004] JHHMMSS.ss+DDMMSS.s> N=23. Table 2: <[DLL2004] MAMBO NTT -MM NNaN> N=82.
=E=	Catalogue in electronic form as J/ApJ/606/664
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EBK2013]
[EBK2013]	(Ellerbroek+Bik+Kaper+, 2013)
Write:	<<[EBK2013] NNN>>
N:	50
Object:	* (SIMBAD class: Star)
Note:	VLT SINFONI (NIR) and VLT X-shooter (optical to NIR) spectroscopy of N=50 stars in RCW 36. Use of Spitzer IRAC archival data.
in source:	RCW 36
Ref:	=2013A&A...558A.102E
by	ELLERBROEK L.E. , BIK A., KAPER L., MAASKANT K.M., PAALVAST M., TRAMPER F., SANA H., WATERS L.B.F.M., BALOG Z.
	Astron. Astrophys., 558A, 102-102 (2013)
	RCW 36 : characterizing the outcome of massive star formation.
o	Table A.1: <[EBK2013] NNN> N=50 among (Nos 1-191).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EBL
EBL	(Extragalactic Background Light)
Write:	<<EBL NNN-N-NNN>>
N:	140+687+644
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST WFPC2 observations: search for EBL sources (Extragalactic Background Light) at F300W, F555W, and F814W bandpasses (300, 555, 814 first 'NNN' in the format). See also [BFM2002]
Ref:	=2002ApJ...571...56B
by	BERNSTEIN R.A. , FREEDMAN W.L., MADORE B.F.
	Astrophys. J., 571, 56-84 (2002)
	The first detections of the extragalactic background light at 3000, 5500, and 8000 Å. I. Results.
o	(Erratum) erratum vol. 632, p. 713 (2005)
o	Table 2: <EBL NNN-N-NNN> N=140+687+644 = <[BFM2002] JHHMMSS.ss-DDMMSS.s> N=140+687+644.
=E=	Catalogue in electronic form as J/ApJ/571/56
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EBL2020]
[EBL2020]	(Emig+Bolatto+Leroy+, 2020)
Write:	<<[EBL2020] NN>>
N:	29
Object:	Poss. Super Cluster of * (SIMBAD class: Cluster*_Candidate = Cluster of Stars Candidate)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 3 (93 GHz/3.2 mm) observations of N=29 bright, compact sources in the central starburst of NGC 4945.
in source:	NGC 4945
Ref:	=2020ApJ...903...50E
by	EMIG K.L. , BOLATTO A.D., LEROY A.K., MILLS E.A.C., JIMENEZ DONAIRE M.J., TIELENS A.G.G.M., GINSBURG A., GORSKI M., KRIEGER N., LEVY R.C., MEIER D.S., OTT J., ROSOLOWSKY E., THOMPSON T.A., VEILLEUX S.
	Astrophys. J., 903, 50-50 (2020)
	Super star clusters in the central starburst of NGC 4945.
o	Fig. 3, Table 1: <[EBL2020] NN> (Nos 1-29).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EBLM
EBLM	(Eclipsing Binaries with Low Mass)
Write:	<<EBLM JHHMM+DD>>
N:	∼500
Object:	EB*Algol (SIMBAD class: EclBin = Eclipsing Binary)
Note:	The EBLM project is an offshoot from the WASP, planet search program. Planets and low mass stars (under 0.2 solar mass) produce similar photometric eclipses when they pass in front of solar type, main sequence stars. While the planets are being published with a WASP indicative, we will publish the binaries under an EBLM name. Two papers were already published (Triaud et al. 2013A&A...549A..18T, Gomez Maqueo Chew et al. 2014A&A...572A..50G) but did not use this notation. The first paper contains a good description of our goals, the two most important being a confirmation of the brown dwarf desert, and a mass/radius/luminosity/metallicity relation for stars at the bottom of the main sequence. We have submitted a third paper containing the orbital elements of 118 objects and have another 110ish eclipsing systems under survey. Because of he number of object, we would prefer calling them with a shorter name than the 1SWASP JHHMMSS.ss+DDMMSS.ss that they otherwise would have. It also facilitates our ways to track who will use our results and estimate our impact. A fourth paper, measuring the mass and radii of a saturn-sized low mass star will be submitted within a fortnight. A fifth and sixth paper containing masses and radii are currently under preparation.
Ref:	=2017A&A...604L...6V
by	VON BOETTICHER A. , TRIAUD A.H.M.J., QUELOZ D., GILL S., LENDL M., DELREZ L., ANDERSON D.R., COLLIER CAMERON A., FAEDI F., GILLON M., GOMEZ MAQUEO CHEW Y., HEBB L., HELLIER C., JEHIN E., MAXTED P.F.L., MARTIN D.V., PEPE F., POLLACCO D., SEGRANSAN D., SMALLEY B., UDRY S., WEST R.
	Astron. Astrophys., 604L, 6-6 (2017)
	The EBLM project. III. A Saturn-size low-mass star at the hydrogen-burning limit.
o	<EBLM JHHMM+DD> (No. J0555-57).
Ref:	=2017A&A...608A.129T
by	TRIAUD A.H.M.J. , MARTIN D.V., SEGRANSAN D., SMALLEY B., MAXTED P.F.L., ANDERSON D.R., BOUCHY F., COLLIER CAMERON A., FAEDI F., GOMEZ MAQUEO CHEW Y., HEBB L., HELLIER C., MARMIER M., PEPE F., POLLACCO D., QUELOZ D., UDRY S., WEST R.
	Astron. Astrophys., 608A, 129-129 (2017)
	The EBLM Project. IV. Spectroscopic orbits of over 100 eclipsing M dwarfs masquerading as transiting hot Jupiters.
o	<EBLM JHHMM+DD> N=118.
Ref:	=2019A&A...625A.150V
by	VON BOETTICHER A. , TRIAUD A.H.M.J., QUELOZ D., GILL S., MAXTED P.F.L., ALMLEAKY Y., ANDERSON D.R., BOUCHY F., BURDANOV A., COLLIER CAMERON A., DELREZ L., DUCROT E., FAEDI F., GILLON M., GOMEZ MAQUEO CHEW Y., HEBB L., HELLIER C., JEHIN E., LENDL M., MARMIER M., MARTIN D.V., McCORMAC J., PEPE F., POLLACCO D., SEGRANSAN D., SMALLEY B., THOMPSON S., TURNER O., UDRY S., VAN GROOTEL V., WEST R.
	Astron. Astrophys., 625A, 150-150 (2019)
	EBLM Project. V. Physical properties of ten fully convective, very-low-mass stars.
o	<EBLM JHHMM+DD> N=10.
Ref:	=2019A&A...626A.119G
by	GILL S. , MAXTED P.F.L., EVANS J.A., EVANS D.F., SOUTHWORTH J., SMALLEY B., GARY B.L., ANDERSON D.R., BOUCHY F., CAMERON A.C., DOMINIK M., FAEDI F., GILLON M., GOMEZ MAQUEO CHEW Y., HEBB L., HELLIER C., JORGENSEN U.G., LONGA-PENA P., MARTIN D.V., McCORMAC J., PEPE F.V., POLLACO D., QUELOZ D., SEGRANSAN D., SNODGRASS C., TURNER O.D., TRIAUD A.H.M., UDRY S., WEST R.G.
	Astron. Astrophys., 626A, 119-119 (2019)
	The EBLM project. VI. Mass and radius of five low-mass stars in F+M binaries discovered by the WASP survey.
o	<EBLM JHHMM+DD> N=5.
o	Paragraph 4.2 Gaia DR2 6539811294185397120 not found in the catalogue. Paragraph 4.3 Gaia DR2 4971670729566470528 not found in the catalogue. Paragraph 4.4 Gaia DR2 2098283457595740288 not found in the catalogue.
Ref:	=2020MNRAS.497.1627K
by	KUNOVAC HODZIC V. , TRIAUD A.H.M.J., MARTIN D.V., FABRYCKY D.C., CEGLA H.M., COLLIER CAMERON A., GILL S., HELLIER C., KOSTOV V.B., MAXTED P.F.L., OROSZ J.A., PEPE F., POLLACCO D., QUELOZ D., SEGRANSAN D., UDRY S., WELSH W.F.
	Mon. Not. R. Astron. Soc., 497, 1627-1633 (2020)
	The EBLM project - VII. Spin-orbit alignment for the circumbinary planet host EBLM J0608-59 A/TOI-1338 A.
o	<EBLM JHHMM+DD> (No. J0608-59). Institute of Astronomy
=E=	Catalogue in electronic form as J/A+A/604/L6
=E=	Catalogue in electronic form as <J/A+A/625/A150/>
=E=	Catalogue in electronic form as <J/A+A/626/A119/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [EBM2012]
[EBM2012]	(Emonts+Burnett+Morganti+, 2012)
Write:	<<[EBM2012] Cloud A>>
N:	2
Object:	HI Cloud (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	WSRT HI observations of N=2 clouds of HI gas in the field of NGC 3801.
Ref:	=2012MNRAS.421.1421E
by	EMONTS B.H.C. , BURNETT C., MORGANTI R., STRUVE C.
	Mon. Not. R. Astron. Soc., 421, 1421-1430 (2012)
	Classical radio source propagating into outer H I disc in NGC 3801.
o	Fig. 5, Table 2: <[EBM2012] Cloud A> (Nos A-B).
o	Clump C in NGC 3801 is not in Simbad.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EBS2006]
[EBS2006]	(Eckart+Baganoff+Schodel+, 2006)
Write:	<<[EBS2006] DN>> <<[EBS2006] D23>> <<[EBS2006] D3.1>>
N:	10+1
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT NACO and SINFONI NIR observations of dust components around Sgr A*.
in source:	NAME Gal Center
Ref:	=2006A&A...450..535E
by	ECKART A. , BAGANOFF F.K., SCHOEDEL R., MORRIS M., GENZEL R., BOWER G.C., MARRONE D., MORAN J.M., VIEHMANN T., BAUTZ M.W., BRANDT W.N., GARMIRE G.P., OTT T., TRIPPE S., RICKER G.R., STRAUBMEIER C., ROBERTS D.A., YUSEF-ZADEH F., ZHAO J.H., RAO R.
	Astron. Astrophys., 450, 535-555 (2006)
	The flare activity of Sagittarius A. New coordinated mm to X-ray* observations.
o	Fig.14: <[EBS2006] DN> (Nos D1-D8).
Ref:	=2020A&A...634A..35P
by	PEISSKER F. , HOSSEINI S.E., ZAJACEK M., ECKART A., SAALFELD R., VALENCIA-S M., PARSA M., KARAS V.
	Astron. Astrophys., 634A, 35-35 (2020)
	Monitoring dusty sources in the vicinity of Sagittarius A.*
o	Fig. 1: <[EBS2006] DNN.N> (Nos D23, D3.1, D9) added, <[MES2007] XN.N> (No. X7.1) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EBS2011]
[EBS2011]	(Erb+Bogosavljevic+Steidel, 2011)
Write:	<<[EBS2011] BLOB N>>
N:	6
Object:	Lyman Alpha Blob (SIMBAD class: EmObj = Emission Object)
Stat:	is completely incorporated in Simbad
Note:	Search for Lyα emitters using deep, narrowband imaging centered at 4010 Angstrom from the Large Format Camera Wide-Field Imager on the Hale 200 inch telescope at Palomar Observatory.
in source:	NAME HS 1700+64 Protocluster
Ref:	=2011ApJ...740L..31E
by	ERB D.K. , BOGOSAVLJEVIC M., STEIDEL C.C.
	Astrophys. J., 740L, 31 (2011)
	Filamentary large-scale structure traced by six Lyα blobs at z = 2.3.
o	Fig. 1, Table 1: <[EBS2011] BLOB N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EBT2011]
[EBT2011]	(Efremova+Bianchi+Thilker+, 2011) (Not yet in Simbad)
Write:	<<[EBT2011] EB-FUV NN>> <<[EBT2011] EB-Ha NN>>
N:	77+39
Object:	Star Forming Region (SIMBAD class: PartofG = Part of a Galaxy)
Note:	N=77 (FUV) and N=39 (Hα) star-forming regions in NGC 6822. Use of GALEX images and of a CTIO Hα image (Massey et al. 2007AJ....134.2474M).
in source:	NGC 6822
Ref:	=2011ApJ...730...88E
by	EFREMOVA B.V. , BIANCHI L., THILKER D.A., NEILL J.D., BURGARELLA D., WYDER T.K., MADORE B.F., REY S.-C., BARLOW T.A., CONROW T., FORSTER K., FRIEDMAN P.G., MARTIN D.C., MORRISSEY P., NEFF S.G., SCHIMINOVICH D., SEIBERT M., SMALL T.
	Astrophys. J., 730, 88 (2011)
	The recent star formation in NGC 6822: an ultraviolet study.
o	Fig. 1, Table 1: <[EBT2011] EB-FUV NN> (Nos 1-77). Fig. 1, Table 2: <[EBT2011] EB-Ha NN> (Nos 1-39).
=E=	Catalogue in electronic form as <J/ApJ/730/88/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EBU2007]
[EBU2007]	(Evans+Bresolin+Urbaneja+, 2007)
Write:	<<[EBU2007] NN>>
N:	91
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 spectroscopic observations of NGC 3109.
in source:	NGC 3109
Ref:	=2007ApJ...659.1198E
by	EVANS C.J. , BRESOLIN F., URBANEJA M.A., PIETRZYNSKI G., GIEREN W., KUDRITZKI R.-P.
	Astrophys. J., 659, 1198-1211 (2007)
	The ARAUCARIA project: VLT-FORS spectroscopy of blue supergiants in NGC 3109. Classifications, first abundances, and kinematics.
o	Table 2: <[EBU2007] NN> (Nos 1-91).
=E=	Catalogue in electronic form as J/ApJ/659/1198
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EBW2018]
[EBW2018]	(Eftekhari+Berger+Williams+, 2018)
Write:	<<[EBW2018] JHHMMSS.sss+DDMMSS.ss>>
N:	5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	JVLA 6GHz continuum and Magellan 6.5m Baade telescope IMACS observations of N=5 radio sources in the field of FRB 170107.
Ref:	=2018ApJ...860...73E
by	EFTEKHARI T. , BERGER E., WILLIAMS P.K.G., BLANCHARD P.K.
	Astrophys. J., 860, 73-73 (2018)
	Associating fast radio bursts with extragalactic radio sources: general methodology and a search for a counterpart to FRB 170107.
o	Fig. 4, Table 2: <[EBW2018] JHHMMSS.sss+DDMMSS.ss> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EC
EC	(Edinburgh-Cape survey)
Write:	<<EC HHMMm-DDMMa>>
N:	20+775+329+892+362+574+179
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	The Edinburgh-Cape (EC) blue object survey. The blue stellar objects are selected by automated techniques from U and B pairs of UK Schmidt Telescope plates scanned with the COSMOS measuring machine. Follow-up photometry and spectroscopy is obtained with the SAAO telescopes.
Ref:	=1991MNRAS.248..664K
by	KILKENNY D. , O'DONOGHUE D., STOBIE R.S.
	Mon. Not. R. Astron. Soc., 248, 664-669 (1991)
	First results from the Edinburgh-Cape faint blue object survey - normal stars at high galactic latitudes.
o	First ref. from this survey. In this ref. <EC HHMMm-DDMM> N=20
Ref:	=1997MNRAS.287..867K
by	KILKENNY D. , O'DONOGHUE D., KOEN C., STOBIE R.S., CHEN A.
	Mon. Not. R. Astron. Soc., 287, 867-893 (1997)
	The Edinburgh-Cape Blue Object Survey - II. Zone 1 - the North Galactic Cap.
o	Tables 1-2: <EC HHMMm-DDMM> N=775+329.
Ref:	=2013MNRAS.431..240O
by	O'DONOGHUE D. , KILKENNY D., KOEN C., HAMBLY N., MacGILLIVRAY H., STOBIE R.S.
	Mon. Not. R. Astron. Soc., 431, 240-251 (2013)
	The Edinburgh-Cape Blue Object Survey - III. Zone 2: galactic latitudes -30° > b > -40°.
o	Tables 3-4: <EC HHMMm-DDMM> N=892+362.
o	EC 13471-1256 is a misprint for EC 13471-1258.
Ref:	=2015MNRAS.453.1879K
by	KILKENNY D. , O'DONOGHUE D., WORTERS H.L., KOEN C., HAMBLY N., MacGILLIVRAY H.
	Mon. Not. R. Astron. Soc., 453, 1879-1887 (2015)
	The Edinburgh-Cape Blue Object Survey - IV. Zone 3: Galactic latitudes -40° > b > -50°.
o	Tables 2-3: <EC HHMMm-DDMMa> N=574+179.
=E=	Catalogue in electronic form as J/MNRAS/287/867
=E=	Catalogue in electronic form as J/MNRAS/453/1879
=E=	Catalogue in electronic form as <J/MNRAS/431/240/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EC
EC	(Eiroa+Casali)
*****	Avoid the usage of EC, prefer [EC92]
Origin	of the Acronym: L (1998A&A...330..990G)
Details on Acronym: EC
EC	(Eiroa+Casali)
*****	Avoid the usage of EC, prefer [EC95]
Origin	of the Acronym: L (2003ApJ...596.1064J)
Details on Acronym: EC
EC	(Extended Cluster)
*****	Avoid the usage of EC, prefer M31WFS
Origin	of the Acronym: L (2006ApJ...653L.105M)
Details on Acronym: [EC2003]
[EC2003]	(Edge+Coe, 2003)= ([EC2003a])
Write:	<<[EC2003] AX J0049.4-7323 JHHMMSS.s+DDMMSS.s>> <<[EC2003] AX J0057.4-7325 A>> <<[EC2003] RX J0101.0-7206 Object N>>
N:	12+5+2
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	SAAO observations and 2MASSi, OGLE data. Search for possible optical counterparts of X-ray sources.
Ref:	=2003MNRAS.338..428E
by	EDGE W.R.T. , COE M.J.
	Mon. Not. R. Astron. Soc., 338, 428-432 (2003)
	Optical counterparts to four X-ray sources in the Small Magellanic Cloud.
o	Abstract: RX J0101.1-7206 is a misprint for RX J0101.0-7206
o	Table 1, Fig.1: <[EC2003] AX J0049.4-7323 JHHMMSS.s+DDMMSS.s> N=12. Table 2, Fig.1: <[EC2003] AX J0057.4-7325 A> (Nos A-E). Fig.5: <[EC2003] RX J0101.0-7206 Object N> (Nos 1, 4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EC2003a]
[EC2003a]	(Edge+Coe, 2003)
*****	Avoid the usage of [EC2003a], prefer [EC2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EC2003b]
[EC2003b]	(Eisner+Carpenter, 2003)
Write:	<<[EC2003b] NN>>
N:	13
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Images of NGC 2024 in 3mm continuum emission with OVRO.
in source:	NGC 2024
Ref:	=2003ApJ...598.1341E
by	EISNER J.A. , CARPENTER J.M.
	Astrophys. J., 598, 1341-1349 (2003)
	Distribution of circumstellar disk masses in the young cluster NGC 2024.
o	Table 1, col(source): FIR N = [MCK88] NGC 2024 FIR N in SIMBAD, IRS N = [BCB89] IRS N.
o	Table 1: <[EC2003b] NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EC2006]
[EC2006]	(Eisner+Carpenter, 2006)= (MM)
Write:	<<[EC2006] MMNN>>
N:	24
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Sources detected in 3mm continuum at Owens Valley Radio Observatory in Orion Nebula Cluster.
in source:	NAME ONC
Ref:	=2006ApJ...641.1162E
by	EISNER J.A. , CARPENTER J.M.
	Astrophys. J., 641, 1162-1171 (2006)
	Massive protoplanetary disks in the Trapezium region.
o	Table 1: <[EC2006] MMNN> (Nos MM01 to MM20).
Ref:	=2008ApJ...683..304E
by	EISNER J.A. , PLAMBECK R.L., CARPENTER J.M., CORDER S.A., QI C., WILNER D.
	Astrophys. J., 683, 304-320 (2008)
	Proplyds and massive disks in the Orion nebula cluster imaged with CARMA and SMA.
o	Table 1: <[EC2006] MMNN> (Nos MM21 to MM24) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EC89]
[EC89]	(Eiroa+Casali, 1989)= (SVS)
Write:	<<[EC89] SVS 4-NN>>
N:	11
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	IRCAM UKIRT observations. N=11 stellar objects in the [SVS76] Ser 4 image.
in source:	NAME Serpens Cloud
Ref:	=1989A&A...223L..17E
by	EIROA C. , CASALI M.M.
	Astron. Astrophys., 223, 17-19 (1989)
	The Serpens sources SVS 4 and FIRS 1 : new results from infrared images.
o	SVS 4 = [SVS76] Ser 4, FIRS 1 = [HWJ84] FIRS 1
o	Table 1: <[EC89] SVS 4-NN> (Nos 4-1 to 4-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EC90]
[EC90]	(Eisenhardt+Chorkshi, 1990)
Write:	<<[EC90] 3C NNN a>>
N:	3+4+4
Object:	Knot (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Components of N=3 3C radio-sources. See [LH88]
Ref:	=1990ApJ...351L...9E
by	EISENHARDT P. , CHOKSHI A.
	Astrophys. J., 351, 9-13 (1990)
	Infrared images of distant 3C radio galaxies.
o	Table 1, Figs: Components 'a' in 3C 194, 3C 437, and 3C 454.1 are '[LH88]' in SIMBAD.
o	Table 1, Figs: <[EC90] 3C 54 a> (Nos a-c), <[EC90] 3C 356 a> (Nos a-d), <[EC90] 3C 441 a> (Nos a-c).
Ref:	=1998MNRAS.298..966L
by	LACY M. , RAWLINGS S., BLUNDELL K.M., RIDGWAY S.E.
	Mon. Not. R. Astron. Soc., 298, 966-976 (1998)
	A radio-jet-galaxy interaction in 3C 441.
o	Fig.1: <[EC90] 3C 441 a> (No. d) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EC92]
[EC92]	(Eiroa+Casali, 1992)= (EC) = (HCE) = (IRS) = (Ser-EC)
Write:	<<[EC92] NNN>>
N:	177
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	In ref. 1997A&A...320L..41H, Table 3: (Nos 164-177) added. In table 2, 10 various [EC92] sources are studied. Some authors have re-numbered these sources 'HCE NN'. HCE acronym is not used in SIMBAD.
in source:	NAME Serpens Cloud
Ref:	=1992A&A...262..468E
by	EIROA C. , CASALI M.M.
	Astron. Astrophys., 262, 468-None (1992)
	Near-infrared images of the Serpens cloud core: the stellar cluster.
o	<[EC92] NNN> N=163
Ref:	=1997A&A...320L..41H
by	HORROBIN M.J. , CASALI M.M., EIROA C.
	Astron. Astrophys., 320, 41-43 (1997)
	Variability and a vanishing YSO in the Serpens cloud core.
o	Table 2: <[EC92] NNN> (Nos 164-177)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EC95]
[EC95]	(Eiroa+Casali, 1995)= (EC)
Write:	<<[EC95] NNN>>
N:	100
Object:	* (SIMBAD class: Star)
in source:	SH 2-269
Ref:	=1995A&A...303...87E
by	EIROA C. , CASALI M.M.
	Astron. Astrophys., 303, 87-94 (1995)
	The S 269 stellar cluster.
o	S269 = SH 2-269
o	Table 1: <[EC95] NNN> (Nos 1-100)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ECB2002]
[ECB2002]	(Eck+Cowan+Branch, 2002)
Write:	<<[ECB2002] NGC NNNN ggg>> <<[ECB2002] NGC NNNNW ggg>> <<[ECB2002] NGC NNNN C>> <<[ECB2002] IC NNNN ggg>>
N:	67
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Non-SN radio-sources in 10 galaxy fields.
Ref:	=2002ApJ...573..306E
by	ECK C.R. , COWAN J.J., BRANCH D.
	Astrophys. J., 573, 306-323 (2002)
	A search for radio emission from supernovae with ages from about 1 week to more than 80 years.
o	Table 5, Figs 6-9: <[ECB2002] NGC NNNN aaa>, <[ECB2002] NGC NNNNW aaa>, <[ECB2002] NGC NNNN A>, <[ECB2002] IC NNNN aaa>, N=67.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ECB2017]
[ECB2017]	(Ellingsen+Chen+Breen+, 2017)
Write:	<<[ECB2017] A>>
N:	7
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	ATCA HC3N line observations of NGC 253.
in source:	NGC 253
Ref:	=2017ApJ...841L..14E
by	ELLINGSEN S.P. , CHEN X., BREEN S.L., QIAO H.-H.
	Astrophys. J., 841L, 14-14 (2017)
	Detection of HC_{3}N maser emission in NGC 253.
o	Table 1: <[ECB2017] A> (Nos A-G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ECD2009]
[ECD2009]	(Eales+Chapin+Devlin+, 2009)
Write:	<<[ECD2009] DD.ddddd+DD.ddddd>> <<[ECD2009] Rad DDD.ddddd+DD.ddddd>> <<[ECD2009] IR DDD.ddddd+DD.ddddd>>
N:	317
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	Balloon-borne Large Aperture Submillimeter Telescope (BLAST) redshift survey at 250, 350 and 500µm in the GOODS SOUTH FIELD. See also BLAST, [DAB2009].
in source:	NAME GOODS South Field
Ref:	=2009ApJ...707.1779E
by	EALES S. , CHAPIN E.L., DEVLIN M.J., DYE S., HALPERN M., HUGHES D.H., MARSDEN G., MAUSKOPF P., MONCELSI L., NETTERFIELD C.B., PASCALE E., PATANCHON G., RAYMOND G., REX M., SCOTT D., SEMISCH C., SIANA B., TRUCH M.D.P., VIERO M.P.
	Astrophys. J., 707, 1779-1808 (2009)
	BLAST: the redshift survey.
o	Table 1: <[ECD2009] Rad DDD.ddddd+DD.ddddd>, <[ECD2009] IR DDD.ddddd+DD.ddddd>. Table 3: <[ECD2009] DD.ddddd+DD.ddddd> N=316.
=E=	Catalogue in electronic form as <J/ApJ/707/1779/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ECD2011]
[ECD2011]	(Enoch+Corder+Duchene+, 2011)
Write:	<<[ECD2011] Ser-emb NN(W)>>
N:	5
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	CARMA 230GHz observations of the Serpens Molecular Cloud. See also [EES2009].
in source:	NAME Serpens Cloud
Ref:	=2011ApJS..195...21E
by	ENOCH M.L. , CORDER S., DUCHENE G., BOCK D.C., BOLATTO A.D., CULVERHOUSE T.L., KWON W., LAMB J.W., LEITCH E.M., MARRONE D.P., MUCHOVEJ S.J., PEREZ L.M., SCOTT S.L., TEUBEN P.J., WRIGHT M.C.H., ZAUDERER B.A.
	Astrophys. J., Suppl. Ser., 195, 21 (2011)
	Disk and envelope structure in class 0 protostars. II. High-resolution millimeter mapping of the Serpens sample.
o	Table 2: <[ECD2011] Ser-emb NN(W)> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ECF2018]
[ECF2018]	(Epinat+Contini+Finley+, 2018)
Write:	<<[ECF2018] A>> <<[ECF2018] NNN>>
N:	9+14
Object:	Region + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	MUSE observations of N=9 extended gas regions and N=14 galaxies in the galaxy group [KLI2012] 30.
in source:	[KLI2012] 30
Ref:	=2018A&A...609A..40E
by	EPINAT B. , CONTINI T., FINLEY H., BOOGAARD L.A., GUEROU A., BRINCHMANN J., CARTON D., MICHEL-DANSAC L., BACON R., CANTALUPO S., CAROLLO M., HAMER S., KOLLATSCHNY W., KRAJNOVIC D., MARINO R.A., RICHARD J., SOUCAIL G., WEILBACHER P.M., WISOTZKI L.
	Astron. Astrophys., 609A, 40-40 (2018)
	Ionised gas structure of 100 kpc in an over-dense region of the galaxy group COSMOS-Gr30 at z ~ 0.7.
o	Fig. 3, Tables 1-3: <[ECF2018] A> (Nos A-I), <[ECF2018] NNN> N=14 among (Nos 57-228).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ECF2022]
[ECF2022]	(Escudero+Cortesi+Faifer+, 2022)
Write:	<<[ECF2022] JDDD.ddddd+DD.ddddd>>
N:	51
Object:	Poss. GlCl (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Gemini-North GMOS observations of N=51 globular cluster candidates in NGC 4382.
in source:	M 85 = NGC 4382
Ref:	=2022MNRAS.511..393E
by	ESCUDERO C.G. , CORTESI A., FAIFER F.R., SESTO L.A., SMITH CASTELLI A.V., JOHNSTON E.J., REYNALDI V., CHIES-SANTOS A.L., SALINAS R., MENENDEZ-DELMESTRE K., GONCALVES T.S., GROSSI M., MENDES DE OLIVEIRA C.
	Mon. Not. R. Astron. Soc., 511, 393-412 (2022)
	The complex globular cluster system of the S0 galaxy NGC 4382 in the outskirts of the Virgo Cluster.
o	Table 5: <[ECF2022] JDDD.ddddd+DD.ddddd> N=51.
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [ECG2005]
[ECG2005]	(Etoka+Cohen+Gray, 2005) (Not yet in Simbad)
Write:	<<[ECG2005] OH NN>> <<[ECG2005] CH3OH NN>>
N:	42+15
Object:	OH + CH3OH Maser (SIMBAD class: Maser)
Note:	MERLIN measurements of OH and CH3OH masers.
Ref:	=2005MNRAS.360.1162E
by	ETOKA S. , COHEN R.J., GRAY M.D.
	Mon. Not. R. Astron. Soc., 360, 1162-1170 (2005)
	The association of OH and methanol masers in W3(OH).
o	Table 1: <[ECG2005] OH NN> (Nos 1-42). Table 2: <[ECG2005] CH3OH NN> (Nos 1-15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ECG2019]
[ECG2019]	(Evans+Castro+Gonzalez+, 2019)
Write:	<<[ECG2019] LP NN>> <<[ECG2019] JHHMMSS.ss+DDMMSS.ss>>
N:	32+2
Object:	* + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	VLT MUSE observations of N=32 confirmed and candidate blue stars and N=2 background galaxies in the Leo P field. Use of HST data.
in source:	NAME Leo P
Ref:	=2019A&A...622A.129E
by	EVANS C.J. , CASTRO N., GONZALEZ O.A., GARCIA M., BASTIAN N., CIONI M.-R.L., CLARK J.S., DAVIES B., FERGUSON A.M.N., KAMANN S., LENNON D.J., PATRICK L.R., VINK J.S., WEISZ D.R.
	Astron. Astrophys., 622A, 129-129 (2019)
	First stellar spectroscopy in Leo P.
o	Table 1: <[ECG2019] LP NN> (Nos 1-32). Table 3: <[ECG2019] JHHMMSS.ss+DDMMSS.ss> N=2.
o	Tables 1,2,3 objects [MSB2013] not in SIMBAD.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ECHA
ECHA	(Eta Chamaeleontis cluster)
Write:	<<ECHA JHHMM.m+DDMM>>
N:	6
Object:	* in Cl* (SIMBAD class: Star)
Note:	N=6 members of Eta Cha Cluster.
in source:	NAME eta Cha Cluster
Ref:	=2002MNRAS.329L..29L
by	LAWSON W.A. , CRAUSE L.A., MAMAJEK E.E., FEIGELSON E.D.
	Mon. Not. R. Astron. Soc., 329, 29-33 (2002)
	ECHA J0843.3-7905: Discovery of an `old' classical T Tauri star in the η Chamaeleontis cluster.
o	Table 1: Anonymous star = EQ J084834.9-785352.
o	Table 1: <ECHA JHHMM.m+DDMM> N=2.
Ref:	=2004ApJ...600.1016S
by	SONG I. , ZUCKERMAN B., BESSELL M.S.
	Astrophys. J., 600, 1016-1019 (2004)
	Probing the low-mass stellar end of the η Chamaeleontis cluster.
o	Table 2: <ECHA JHHMM.m+DDMM> N=4 added.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ECHA
ECHA	(Eta Chamaeleontis cluste)
*****	Avoid the usage of ECHA, prefer RECX
Origin	of the Acronym: L (2008ApJ...683..813G)
Details on Acronym: [ECM2002]
[ECM2002]	(Elmegreen+Chromey+McGrath+, 2002) (Not yet in Simbad)
Write:	<<[ECM2002] NNN>> <<[ECM2002] A>>
N:	118+4
Object:	Core + Region (SIMBAD class: PartofG = Part of a Galaxy)
Note:	N=118 cores in NGC 3310, among which 17 are Super Star Clusters. N=4 star forming regions.
in source:	NGC 3310
Ref:	=2002AJ....123.1381E
by	ELMEGREEN D.M. , CHROMEY F.R., McGRATH E.J., OSTENSON J.M.
	Astron. J., 123, 1381-1388 (2002)
	Circumnuclear star formation in the spiral galaxy NGC 3310.
o	Fig.2, Table 2: <[ECM2002] NNN> (Nos 1-118), [ECM2002] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ECM2006]
[ECM2006]	(Eigenbrod+Courbin+Meylan+, 2006)
Write:	<<[ECM2006] HE 0230-2130 GN>> <<[ECM2006] SDSS JHHMM+DDMM>> <<[ECM2006] SDSS JHHMM+DDMM A>>
N:	2+2+5+3
Object:	Grav. lensed image + G (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	VLT FORS observations. Measure of the redshift of lensing galaxies of gravitationally lensed QSOs: HE 0230-2130: see [WCL99] for the 4 lensed images A to D, a main lensing galaxy G1 and a second one G2 are found. QSO J1138+0314: 4 lensing images A to D and a lensing galaxy G are found. QSO J1226-0006: 2 lensing images A, B and a lensing galaxy G are found.
Ref:	=2006A&A...451..759E
by	EIGENBROD A. , COURBIN F., MEYLAN G., VUISSOZ C., MAGAIN P.
	Astron. Astrophys., 451, 759-766 (2006)
	COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses. III. Redshift of the lensing galaxy in eight gravitationally lensed quasars.
o	Fig.2, text: <[ECM2006] HE 0230-2130 GN> (Nos G1-G2). Fig.4, text: <[ECM2006] SDSS J1138+0314> N=1, <[ECM2006] SDSS J1138+0314 A> (Nos A-D, G). Fig.5, text: <[ECM2006] SDSS J1226-0006> N=1, <[ECM2006] SDSS J1226-0006 A> (Nos A-B, G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ECM85]
[ECM85]	(Ellis+Couch+MacLaren+, 1985)
Write:	<<[ECM85] NNN>>
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Table 5: G in ClG 0016+16, same numbering as '[AEC93] 0016+16 NNN'. See also CN
in source:	ClG 0016+1609 = 1E 0015.9+1609
Ref:	=1985MNRAS.217..239E
by	ELLIS R.S. , COUCH W.J., MacLAREN I., KOO D.C.
	Mon. Not. R. Astron. Soc., 217, 239-264 (1985)
	Spectral energy distributions for galaxies in high-redshift clusters - II. 0016+16 at z = 0.54.
o	Table 5: <[ECM85] NNN> = <CN C0016+16 NNN>, N=47 among 150.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ECO
ECO	(Environmental COntext catalog)
Write:	<<ECO NNNNN>>
N:	12681+37
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Environmental COntext, catalog of N=12681 galaxies. Use of archival UZC catalog and SDSS data.
Ref:	=2015ApJ...812...89M
by	MOFFETT A.J. , KANNAPPAN S.J., BERLIND A.A., ECKERT K.D., STARK D.V., HENDEL D., NORRIS M.A., GROGIN N.A.
	Astrophys. J., 812, 89 (2015)
	ECO and RESOLVE: galaxy disk growth in environmental context.
o	Table 1: <ECO NNNNN> (Nos 1-12681).
Ref:	=2017ApJ...849...20E
by	ECKERT K.D. , KANNAPPAN S.J., LAGOS C.D.P., BAKER A.D., BERLIND A.A., STARK D.V., MOFFETT A.J., NASIPAK Z., NORRIS M.A.
	Astrophys. J., 849, 20-20 (2017)
	The baryonic collapse efficiency of galaxy groups in the RESOLVE and ECO surveys.
o	(Erratum) erratum vol. 920, art. 160 (2021)
o	eco.dat: <ECO NNNNN> N=37 added among (Nos 13683-13883).
=E=	Catalogue in electronic form as J/ApJ/812/89
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ECP2006]
[ECP2006]	(Ekta+Chengalur+Pustilnik, 2006)
Write:	<<[ECP2006] SBSG 1129+577 AN>> <<[ECP2006] AN>> (not recognised by Simbad, but found in literature)
N:	4
Object:	Star Forming Region (SIMBAD class: Region = Region defined in the Sky)
Stat:	is completely incorporated in Simbad
Note:	GMRT HI observations of SBSG 1129+576 and SBSG 1129+577. N=4 star-forming regions in SBSG 1129+577.
in source:	SBSG 1129+577
Ref:	=2006MNRAS.372..853E
by	EKTA , CHENGALUR J.N., PUSTILNIK S.A.
	Mon. Not. R. Astron. Soc., 372, 853-861 (2006)
	HI studies of extremely metal-deficient galaxies - II. Giant Metrewave Radio Telescope observations of SBS 1129+576.
o	Paragr. 4.1: <[ECP2006] SBSG 1129+577 AN> (Nos A1-A4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ECR2004]
[ECR2004]	(Ellison+Churchill+Rix+, 2004)
Write:	<<[ECR2004] QSO JHHMM+DDMM abs N.NNNN>>
N:	57
Object:	Absorber
Note:	CORALS survey to search for absorbers in 35 QSOs.
Ref:	=2004ApJ...615..118E
by	ELLISON S.L. , CHURCHILL C.W., RIX S.A., PETTINI M.
	Astrophys. J., 615, 118-129 (2004)
	The number density of 0.6 < z < 1.7 mg II systems from CORALS: observational biases at intermediate redshift.
o	Table 3: <[ECR2004] QSO JHHMM+DDMM abs N.NNNN> N=57.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ECS97]
[ECS97]	(Elmegreen+Chrmey+Santos+, 1997) (Not yet in Simbad)
Write:	<<[ECS97] NGC 5248 A>> <<[ECS97] NGC 3504 A>> <<[ECS97] NGC 3351 A>>
N:	8+5+9
Object:	Hotspot (SIMBAD class: PartofG = Part of a Galaxy)
in source:	NGC 5248
in source:	NGC 3504
in source:	NGC 3351
Ref:	=1997AJ....114.1850E
by	ELMEGREEN D.M. , CHROMEY F.R., SANTOS M., MARSHALL D.
	Astron. J., 114, 1850-1857 (1997)
	Near-infrared observations of circumnuclear star formation in NGC 3351, NGC 3504, and NGC 5248.
o	Tables 2, 3: <[ECS97] NGC 5248 A> (Nos A-H), <[ECS97] NGC 3504 A> (Nos A-E), <[ECS97] NGC 3351 A> (Nos A-I)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ECS99]
[ECS99]	(Elmegreen+Chromey+Sawyer+, 1999) (Not yet in Simbad)
Write:	<<[ECS99] NGC NNNN Na>>
N:	11+8
Object:	Hot Spot (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Map in Fig.2
in source:	NGC 2997
in source:	NGC 6951
Ref:	=1999AJ....118..777E
by	ELMEGREEN D.M. , CHROMEY F.R., SAWYER J.E., REINFELD E.L.
	Astron. J., 118, 777-784 (1999)
	Near-infrared observations of hot spots in the circumnuclear rings of NGC 2997 and NGC 6951.
o	Table 1: <[ECS99] NGC 2997 Na> (Nos 1-9, 2a, 7a), <[ECS99] NGC 6951 N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ECV2009]
[ECV2009]	(Elvis+Civano+Vignali+, 2009)= (CID)
Write:	<<[ECV2009] NNNNN>>
N:	1761
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	The Chandra COSMOS Survey (C-COSMOS) of the central 0.5 square degrees of the COSMOS field. See also CXOC.
in source:	NAME COSMOS Field
Ref:	=2009ApJS..184..158E
by	ELVIS M. , CIVANO F., VIGNALI C., PUCCETTI S., FIORE F., CAPPELLUTI N., ALDCROFT T.L., FRUSCIONE A., ZAMORANI G., COMASTRI A., BRUSA M., GILLI R., MIYAJI T., DAMIANI F., KOEKEMOER A.M., FINOGUENOV A., BRUNNER H., URRY C.M., SILVERMAN J., MAINIERI V., HASINGER G., GRIFFITHS R., CAROLLO M., HAO H., GUZZO L., BLAIN A., CALZETTI D., CARILLI C., CAPAK P., ETTORI S., FABBIANO G., IMPEY C., LILLY S., MOBASHER B., RICH M., SALVATO M., SANDERS D.B., SCHINNERER E., SCOVILLE N., SHOPBELL P., TAYLOR J.E., TANIGUCHI Y., VOLONTERI M.
	Astrophys. J., Suppl. Ser., 184, 158-171 (2009)
	The Chandra COSMOS survey. I. Overview and point source catalog.
o	Catalog, col(1): <CXOC JHHMMSS.s+DDMMSS> N=1761 = Catalog, col(2): <[ECV2009] NNNNN> N=1761 among (Nos 1-22962).
=E=	Catalogue in electronic form as J/ApJS/184/158
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ECW98]
[ECW98]	(Elmegreen+Chromey+Warren, 1998)
Write:	<<[ECW98] 3-NN>> <<[ECW98] 4-N>>
N:	27+8
Object:	Feature (SIMBAD class: PartofG = Part of a Galaxy)
Note:	IRIM/KPNO observations. Table 3: format '3-NN', N=27 regions of dust features, map in Fig.1. Table 4: format '4-N', N=8 hot spots, No. 1 = nucleus of M 83, map in Fig.8.
in source:	M 83 = NGC 5236
Ref:	=1998AJ....116.2834E
by	ELMEGREEN D.M. , CHROMEY F.R., WARREN A.R.
	Astron. J., 116, 2834-2840 (1998)
	Discovery of a double circumnuclear ring and minibar in the starburst galaxy M83.
o	Table 3: <[ECW98] 3-NN> (Nos 1 to 27). Table 4: <[ECW98] 4-N> (Nos 1 to 8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ECX6-
ECX6-	(Effelsberg obs., Cygnus X, 6cm)
Write:	<<ECX6- NNA>>
N:	47
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Table 4: (Nos 1-41) + N=6 format 'NNA', small diameter sources at 4800MHz
Ref:	=1991A&A...241..551W
by	WENDKER H.J. , HIGGS L.A., LANDECKER T.L.
	Astron. Astrophys., 241, 551-580 (1991)
	The Cygnus X region. XVIII. A detailed investigation of radio-continuum structure on large and small scales.
o	Table 2: <18P NNNA> (Nos 1-103), N=109. Table 3: <19P NNA> (Nos 1-48), N=50. Table 4: <EXC6-NNA> (Nos 1-41), N=47. Table 6: <CXR NN> (Nos 1-13), N=13, Table 7: <CXH N> (Nos 1-6), N=6
=E=	Catalogue in electronic form as J/A+A/241/551
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EDA2008]
[EDA2008]	(Eskridge+De Grus+Anders+, 2008)
Write:	<<[EDA2008] NN>>
N:	13
Object:	Poss. Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 and NICMOS observations of NGC 1311.
in source:	NGC 1311
Ref:	=2008AJ....135..120E
by	ESKRIDGE P.B. , DE GRIJS R., ANDERS P., WINDHORST R.A., MAGER V.A., JANSEN R.A.
	Astron. J., 135, 120-129 (2008)
	Star clusters in the nearby late-type galaxy NGC 1311.
o	Table 3: <[EDA2008] NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EDCC
EDCC	(Edinburgh-Durham Cluster Catalogue)
Write:	<<EDCC NNN>>
N:	769
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	Supersedes the ACO catalogue as a data base for statistical studies of cluster properties. Table 3: N=737 among (Nos 1-769) Table 4: N=32 among (Nos 30-760) misidentified as clusters. Primary galaxy data set for the cluster survey is the Edinburgh-Durham Southern Galaxy Catalogue EDSGC.
Ref:	=1992MNRAS.258....1L
by	LUMSDEN S.L. , NICHOL R.C., COLLINS C.A., GUZZO L.
	Mon. Not. R. Astron. Soc., 258, 1-22 (1992)
	The Edinburgh-Durham southern galaxy catalogue. IV. The cluster catalogue.
o	Tables 3, 4: <EDCC NNN> (Nos 1-769)
=E=	Catalogue in electronic form as VII/175
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EDCS
EDCS	(ESO Distant Cluster Survey)= (EDCSN) = (EDCSX) = (EDisCS)
Write:	<<EDCS JHHMMSSs+DDMMSSsA>>
N:	672+259+40957+1385
Object:	G in ClG (SIMBAD class: Galaxy)
Note:	ESO Distant Cluster Survey with the FORS2 spectrograph on the VLT, for 20 clusters.
Ref:	=2004A&A...427..397H
by	HALLIDAY C. , MILVANG-JENSEN B., POIRIER S., POGGIANTI B.M., JABLONKA P., ARAGON-SALAMANCA A., SAGLIA R.P., DE LUCIA G., PELLO R., SIMARD L., CLOWE D.I., RUDNICK G., DALCANTON J.J., WHITE S.D.M., ZARITSKY D.
	Astron. Astrophys., 427, 397-413 (2004)
	Spectroscopy of clusters in the ESO Distant Cluster Survey (EDisCS). Redshifts, velocity dispersions and substructure for 5 clusters.
o	Membership probability in Simbad comes from the membership flag given in tables: flag "1", for cluster members within 3 σ cluster of the cluster redshift, has been interpreted into 100%; flag "2", for galaxies at 3 to 4 σ cluster from the cluster redshift, has been interpreted into 80%; flag "3", for galaxies at 4 to 10 σ cluster from the cluster redshift, has been interpreted into 50%; flag "0", for fore- or background galaxies, has been interpreted into O%.
o	Catalogues: <EDCS JHHMMSSs+DDMMSSsA> N=158+128+131+136+119.
Ref:	=2005ApJ...630..206F
by	FINN R.A. , ZARITSKY D., McCARTHY D.W.Jr, POGGIANTI B., RUDNICK G., HALLIDAY C., MILVANG-JENSEN B., PELLO R., SIMARD L.
	Astrophys. J., 630, 206-227 (2005)
	Hα-derived star formation rates for three z≃0.75 EDisCS galaxy clusters.
o	Tables 3, 4, 5: <EDCS JHHMMSSs+DDMMSSsA> N=41+71+147.
Ref:	=2005A&A...444..365W
by	WHITE S.D.M. , CLOWE D.I., SIMARD L., RUDNICK G., DE LUCIA G., ARAGON-SALAMANCA A., BENDER R., BEST P., BREMER M., CHARLOT S., DALCANTON J., DANTEL M., DESAI V., FORT B., HALLIDAY C., JABLONKA P., KAUFFMANN G., MELLIER Y., MILVANG-JENSEN B., PELLO R., POGGIANTI B., POIRIER S., ROETTGERING H., SAGLIA R., SCHNEIDER P., ZARITSKY D.
	Astron. Astrophys., 444, 365-379 (2005)
	EDisCS - the ESO distant cluster survey. Sample definition and optical photometry.
o	Catalog: <EDCS JHHMMSSs+DDMMSSsA> N=40957.
Ref:	=2008A&A...482..419M
by	MILVANG-JENSEN B. , NOLL S., HALLIDAY C., POGGIANTI B.M., JABLONKA P., ARAGON-SALAMANCA A., SAGLIA R.P., NOWAK N., VON DER LINDEN A., DE LUCIA G., PELLO R., MOUSTAKAS J., POIRIER S., BAMFORD S.P., CLOWE D.I., DALCANTON J.J., RUDNICK G.H., SIMARD L., WHITE S.D.M., ZARITSKY D.
	Astron. Astrophys., 482, 419-449 (2008)
	Spectroscopy of clusters in the ESO distant cluster survey (EDisCS). II. Redshifts, velocity dispersions, and substructure for clusters in the last 15 fields.
o	Catalog main+supp: <EDCS JHHMMSSs+DDMMSSsA> N=1319+66. Table 5: <[MNH2008] cl JHHMM.m+DDMMa> N=21.
=E=	Catalogue in electronic form as J/A+A/427/397
=E=	Catalogue in electronic form as J/ApJ/630/206
=E=	Catalogue in electronic form as J/A+A/444/365
=E=	Catalogue in electronic form as J/A+A/482/419
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EDCSN
EDCSN	(ESO Distant Cluster Survey, N)
*****	Avoid the usage of EDCSN, prefer EDCS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EDCSX
EDCSX	(ESO Distant Cluster Survey, X)
*****	Avoid the usage of EDCSX, prefer EDCS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EDG2007]
[EDG2007]	(Eisenhardt+De Propris+Gonzalez+, 2007)
Write:	<<[EDG2007] NNN>>
N:	745
Object:	Unknown (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	KPNO 1.4m telescope NIR and 0.4m telescope optical photometry of J+H band-selected objects in a region centered on the core of the Coma Cluster.
in source:	Coma Cluster = ACO 1656
Ref:	=2007ApJS..169..225E
by	EISENHARDT P.R. , DE PROPRIS R., GONZALEZ A.H., STANFORD S.A., WANG M., DICKINSON M.
	Astrophys. J., Suppl. Ser., 169, 225-238 (2007)
	Multiaperture UBVRIzJHK photometry of galaxies in the Coma cluster.
o	Table 1: <[EDG2007] NNN> (Nos 1-745).
=E=	Catalogue in electronic form as J/ApJS/169/225
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EDH2015]
[EDH2015]	(Eger+Domainko+Hahn, 2015) (Not yet in Simbad)
Write:	<<[EDH2015] Suzaku JHHMM.m+DDMM>>
N:	10
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	N=10 X-ray sources, potential counterparts of HESS J1507-622. Use of Suzaku images, and of Chandra and XMM data.
Ref:	=2015MNRAS.447.3564E
by	EGER P. , DOMAINKO W.F., HAHN J.
	Mon. Not. R. Astron. Soc., 447, 3564-3575 (2015)
	Exploring the potential X-ray counterpart of the puzzling TeV γ-ray source HESS J1507-622 with new Suzaku observations.
o	Fig. 1, Table 2: <[EDH2015] Suzaku JHHMM.m+DDMM> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Edinburgh
Edinburgh	(Edinburgh obs.)= (E) (Not yet in Simbad)
Write:	<<Edinburgh N-NNNA>>
N:	1568
Object:	M * + Carbon * (SIMBAD class: Star)
Ref:	=1971PROE....7....1N
by	NANDY K. , SMRIGLIO F.
	Publ. R. Obs. Edinburgh, 7, 1-18 (1971)
	Spectrophotometry of cool stars in the near infrared. 1. Results for a region in Cygnus.
o	Tables 4a-4b: <Edinburgh 1-NNN> (Nos 1-1 to 1-442)
Ref:	=1971PROE....7...73N
by	NANDY K. , SMRIGLIO F.
	Publ. R. Obs. Edinburgh, 7, 73-84 (1971)
	Spectrophotometry of cool stars in the near infrared. II. Results for a region in the direction of the galactic anticentre.
o	Tables 2-3: <Edinburgh 2-NNN> (Nos 2-1 to 2-284)
Ref:	=1976PROE....9..117N
by	NANDY K. , SMRIGLIO F.
	Publ. R. Obs. Edinburgh, 9, 117-123 (1976)
	Spectrophotometry of cool stars in the near infrared. III. Results for a region in the direction of lII=138°.
o	Table 3: <Edinburgh 3-NNN> (Nos 3-1 to 3-284)
Ref:	=1978PROE....9..125N
by	NANDY K. , SMRIGLIO F., BUONANNO R.
	Publ. R. Obs. Edinburgh, 9, 125-134 (1978)
	Spectrophotometry of cool stars in the near infrared. IV. Results for a region in Cassiopeia.
o	Tables 3a-3b: <Edinburgh 4-NNN> (Nos 4-1 to 4-563)
Details on Acronym: EDisCS
EDisCS	(ESO Distant Cluster Survey) (Not yet in Simbad)
*****	Avoid the usage of EDisCS, prefer EDCS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EDJ2007]
[EDJ2007]	(Evstigneeva+Drinkwater+Jurek+, 2007)
Write:	<<[EDJ2007] Dorado N>> <<[EDJ2007] NGC 1400 N>>
N:	3+2
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	AAT spectroscopic observations: search for ultracompact galaxies in galaxy groups.
in source:	NAME DORADO GROUP
in source:	NAME NGC 1400 GROUP
Ref:	=2007MNRAS.378.1036E
by	EVSTIGNEEVA E.A. , DRINKWATER M.J., JUREK R., FIRTH P., JONES J.B., GREGG M.D., PHILLIPPS S.
	Mon. Not. R. Astron. Soc., 378, 1036-1042 (2007)
	Searches for ultracompact dwarf galaxies in galaxy groups.
o	Table 3, Fig.2: <[EDJ2007] Dorado N> (Nos 1-3), <[EDJ2007] NGC 1400 N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EDJ2009]
[EDJ2009]	(Evans+Dunham+Jorgensen+, 2009)
Write:	<<[EDJ2009] NNNN>>
N:	1024
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Spitzer c2d Legacy project observations of 5 nearby molecular clouds to search for YSOs.
in source:	NAME Cha II
in source:	NAME Lupus Cloud
in source:	NAME Perseus Molecular Cloud
in source:	NAME Serpens Cloud
in source:	NAME Ophiuchus Cloud
Ref:	=2009ApJS..181..321E
by	EVANS N.J. , DUNHAM M.M., JORGENSEN J.K., ENOCH M.L., MERIN B., VAN DISHOECK E.F., ALCALA J.M., MYERS P.C., STAPELFELDT K.R., HUARD T.L., ALLEN L.E., HARVEY P.M., VAN KEMPEN T., BLAKE G.A., KOERNER D.W., MUNDY L.G., PADGETT D.L., SARGENT A.I.
	Astrophys. J., Suppl. Ser., 181, 321-350 (2009)
	The Spitzer c2d legacy results: star-formation rates and efficiencies: evolution and lifetimes.
o	Tables 8-12: <[EDJ2009] NNNN> (Nos 1-1024).
=E=	Catalogue in electronic form as J/ApJS/181/321
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EDO
EDO	(?)
*****	Avoid the usage of EDO, prefer COS
Origin	of the Acronym: L = Found in the literature
Details on Acronym: EDO
EDO	(?)
*****	Avoid the usage of EDO, prefer [V67]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: EDON
EDON	(?)
*****	Avoid the usage of EDON, prefer Olsz
Origin	of the Acronym: L = Found in the literature
Details on Acronym: EDS
EDS	(Extended Deep Survey)= (DS)
Write:	<<EDS HHMMSS+DDMMSS>>
N:	25
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Einstein IPC and HRI observations
Ref:	=1991ApJ...374..440P
by	PRIMINI F.A. , MURRAY S.S., HUCHRA J., SCHILD R., BURG R., GIACCONI R.
	Astrophys. J., 374, 440-None (1991)
	The CfA Eisntein observatory extended deep X-ray survey.
o	Table 3: <EDS HHMMSS+DDMMSS> N=25
=E=	Catalogue in electronic form as IX/22
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: EDSGC
EDSGC	(Edinburg-Durham Southern Galaxy Catalog)
Write:	<<EDSGC HHMMSS.s+DDMMSS>>
N:	777
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	The catalog is described in 1989MNRAS.238..379H. In 1995MNRAS.274.1071C: N=777 G in 94 clusters. Objects with no coordinates not in SIMBAD.
Ref:	=1995MNRAS.274.1071C
by	COLLINS C.A. , GUZZO L., NICHOL R.C., LUMSDEN S.L.
	Mon. Not. R. Astron. Soc., 274, 1071-1092 (1995)
	The Edinburgh-Durham Southern Galaxy Catalogue. VII. The Edinburgh-Milano cluster redshift survey.
o	Table 3: <EDSGC HHMMSS.s-DDMMSS> N=777
=E=	Catalogue in electronic form as J/MNRAS/274/1071
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EDXS
EDXS	(ELAIS Deep X-ray Survey)
*****	Avoid the usage of EDXS, prefer [MJA2003]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EDZ97]
[EDZ97]	(Esamdin+Dong+Zhao+, 1997)
Write:	<<[EDZ97] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	Catacl. V* (SIMBAD class: CataclyV* = Cataclysmic Binary)
Stat:	is completely incorporated in Simbad
Ref:	=1997IAUC.6763R...1B
by	BAO SUPERNOVA SURVEY , ESAMDIN A., DONG X., ZHAO Y.
	IAU Circ., 6763, 1-None (1997)
	Cataclysmic variable in Cetus.
o	<[EDZ97] J002727.93-010826.8> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EEB2013]
[EEB2013]	(Ebeling+Edge+Burgett+, 2013)= (eMACS)
Write:	<<[EEB2013] eMACS JHHMM.m+DDMM>> <<[EEB2013] {eMACS} JHHMM.m+DDMM-{g\|x}NN{s}>> <<[EEB2013] RX JHHMM.m+DDMM-gNNs>>
N:	5+165
Object:	Cluster of G + G + (X) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Results of a pilot study for the extended Massive Cluster Survey (eMACS). Keck-II DEIMOS spectroscopy of N=165 sources in the field of five clusters of galaxies.
Ref:	=2013MNRAS.432...62E
by	EBELING H. , EDGE A.C., BURGETT W.S., CHAMBERS K.C., HODAPP K.W., HUBER M.E., KAISER N., PRICE P.A., TONRY J.L.
	Mon. Not. R. Astron. Soc., 432, 62-72 (2013)
	X-ray selected galaxy clusters in the Pan-STARRS Medium Deep Survey.
o	In Table A1, galaxy RX J1613.7+5542-g7 at z=0.3498 is [EEB2013] 1613.7+5542-g9 in SIMBAD; and galaxy RX J1613.7+5542-g7s is [EEB2013] 1613.7+5542-g9s.
o	Table 2: <eMACS JHHMM.m+DDMM> N=5 = <[EEB2013] eMACS JHHMM.m+DDMM> N=5. Table A1: <[EEB2013] eMACS JHHMM.m+DDMM-gNN>, <[EEB2013] eMACS JHHMM.m+DDMM-gNNs>, <[EEB2013] eMACS JHHMM.m+DDMM-xN>, <[EEB2013] RX JHHMM.m+DDMM-gNN>, <[EEB2013] RX JHHMM.m+DDMM-gNNs>, N=165.
=E=	Catalogue in electronic form as <J/MNRAS/432/62/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EEE2014]
[EEE2014]	(Elmegreen+Elmegreen+Erroz-Ferrer+, 2014)
Write:	<<[EEE2014] NGC NNNN NN>>
N:	15+16+12+13+17 (SIMBAD class: StarFormingReg = Star Forming Region)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC observations of nearby spiral galaxies within the S4G survey. Use of SINGS Halpha images.
in source:	NGC 4321
in source:	M 63 = NGC 5055
in source:	M 51 = NGC 5194
in source:	NGC 5248
in source:	M 101 = NGC 5457
Ref:	=2014ApJ...780...32E
by	ELMEGREEN D.M. , ELMEGREEN B.G., ERROZ-FERRER S., KNAPEN J.H., TEICH Y., POPINCHALK M., ATHANASSOULA E., BOSMA A., COMERON S., EFREMOV Yu.N., GADOTTI D.A., GIL DE PAZ A., HINZ J.L., HO L.C., HOLWERDA B., KIM T., LAINE J., LAURIKAINEN E., MENENDEZ-DELMESTRE K., MIZUSAWA T., MUNOZ-MATEOS J.-C., REGAN M.W., SALO H., SEIBERT M., SHETH K.
	Astrophys. J., 780, 32 (2014)
	Embedded star formation in S^{4}G galaxy dust lanes.
o	Table 2: <[EEE2014] NGC NNNN NN> N=15+16+12+13+17.
Details on Acronym: [EEE2018]
[EEE2018]	(Elmegreen+Elmegreen+Efremov, 2018) (Not yet in Simbad)
Write:	<<[EEE2018] JHHMMSS.ssss+DDMMSS.sss>>
N:	147
Object:	Clump (SIMBAD class: Cloud)
Note:	IR images of N=147 clumps in filaments in Messier 100. Use of archival Spitzer IRAC data.
in source:	M 100 = NGC 4321
Ref:	=2018ApJ...863...59E
by	ELMEGREEN B.G. , ELMEGREEN D.M., EFREMOV Y.N.
	Astrophys. J., 863, 59-59 (2018)
	Regularly spaced Infrared peaks in the dusty spirals of Messier 100.
o	Tables 1-2: <[EEE2018] JHHMMSS.ssss+DDMMSS.sss> N=147.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EEF2005]
[EEF2005]	(Elmegreen+Elmegreen+Ferguson, 2005)
Write:	<<[EEF2005] EN>> <<[EEF2005] UDF NNNN Clump N>>
N:	3+8
Object:	G + Clump (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Study of elliptical galaxies in the UDF. 3 Elliptical galaxies not in the UDF catalog are found, (Nos E1-E3). Clumps in 4 UDF galaxies.
Ref:	=2005ApJ...623L..71E
by	ELMEGREEN D.M. , ELMEGREEN B.G., FERGUSON T.E.
	Astrophys. J., 623, 71-74 (2005)
	Central blue clumps in elliptical galaxies of the Hubble Ultra Deep Field.
o	Table 1: <[EEF2005] EN> (Nos E1-E3). Table 2: <[EEF2005] UDF NNNN Clump N> N=2+1+4+1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EEH2003]
[EEH2003]	(Einasto+Einasto+Husti+, 2003)
Write:	<<[EEH2003] -DD.NNa>>
N:	19+4+17+15+18+14+17
Object:	Super Cluster of Galaxies (SIMBAD class: SuperClG = Supercluster of Galaxies)
Note:	Search for superclusters of galaxies in the LCRS. In the format '-DD' stands for declinaison center of 6 slices, 3 in the Northern and 3 in the Southern Galactic Cap. See also [EHE2003] for clusters and groups.
Ref:	=2003A&A...410..425E
by	EINASTO J. , EINASTO M., HUETSI G., SAAR E., TUCKER D.L., TAGO E., MUELLER V., HEINAEMAEKI P., ALLAM S.S.
	Astron. Astrophys., 410, 425-443 (2003)
	Clusters and superclusters in the Las Campanas redshift survey.
o	Tables 5, 6: <[EEH2003] -DD.NNa> N=19+4+17+15+18+14+17.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EEH2004]
[EEH2004]	(Elmegreen+Meloy Elmegreen+Hirst, 2004)
Write:	<<[EEH2004] SN>>
N:	5
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST ACS survey of the field around the Tadpole galaxy. 5 new galaxies are found, not observed in [BFB2004].
Ref:	=2004ApJ...612..191E
by	ELMEGREEN B.G. , ELMEGREEN D.M., HIRST A.C.
	Astrophys. J., 612, 191-201 (2004)
	A constant bar fraction out to redshift z ~ 1 in the advanced camera for surveys field of the tadpole galaxy.
o	Table 1: <[EEH2004] SN> (Nos S1-S5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EEK2006]
[EEK2006]	(Elmegreen+ Elmegreen+Kaufman+, 2006)
Write:	<<[EEK2006] NNN>>
N:	225
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Spitzer Space Telescope IRAC and MIPS observations of the interacting galaxies IC 2163 and NGC 2207: 225 bright emission clumps are observed by IRAC. See also [EKS2000].
in source:	IC 2163
in source:	NGC 2207
Ref:	=2006ApJ...642..158E
by	ELMEGREEN D.M. , ELMEGREEN B.G., KAUFMAN M., SHETH K., STRUCK C., THOMASSON M., BRINKS E.
	Astrophys. J., 642, 158-170 (2006)
	Spitzer Space Telescope IRAC and MIPS observations of the interacting galaxies IC 2163 and NGC 2207: clumpy emission.
o	Table 3: <[EEK2006] NNN> (Nos 1-225).
=E=	Catalogue in electronic form as J/ApJ/642/158
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EER2005]
[EER2005]	(Elmegreen+Elmegreen+Rubin+, 2005)
Write:	<<[EER2005] CNN>> <<[EER2005] CCNN>> <<[EER2005] DNN>> <<[EER2005] TN>> <<[EER2005] sNN>> <<[EER2005] EN>>
N:	12+16+11+8+28+6
Object:	G (SIMBAD class: Galaxy)
Note:	HST ACS images of the HUDF. Galaxies not in the UDF catalog: 12 chains (format CNN), 16 Clump-Clusters (format CCNN), 11 doubles (format DNN), 8 Tadpoles (format TN), 28 spirals (format sNN), and 6 Ellipticals (format EN).
in source:	NAME HUDF
Ref:	=2005ApJ...631...85E
by	ELMEGREEN D.M. , ELMEGREEN B.G., RUBIN D.S., SCHAFFER M.A.
	Astrophys. J., 631, 85-100 (2005)
	Galaxy morphologies in the Hubble Ultra Deep Field: dominance of linear structures at the detection limit.
o	Table 1: <[EER2005] CNN> (Nos C1-C12). Table 2: <[EER2005] CCNN> (Nos CC1-CC16). Table 3: <[EER2005] DNN> (Nos D1-D11). Table 4: <[EER2005] TN> (Nos T1-T8). Table 5: <[EER2005] sNN> (Nos s1-s28). Table 6: <[EER2005] EN> (Nos E1-E6).
=E=	Catalogue in electronic form as J/ApJ/631/85
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EES
EES	(Elston+Eisenhardt+Stanford+)
Write:	<<EES NNN>>
N:	19+1
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Study of G in ClG J0848+4453. The authors refer to a 'EES' catalog in preparation, but never published... See also [RSE99].
in source:	ClG J0848+4453
Ref:	=1997AJ....114.2232S
by	STANFORD S.A. , ELSTON R., EISENHARDT P.R., SPINRAD H., STERN D., DEY A.
	Astron. J., 114, 2232-2239 (1997)
	An IR-selected galaxy cluster at z=1.27.
o	in ref list: Arago-Salamanca 1991MNRAS instead of 1993
o	Table 1: <EES NNN> N=19 among (Nos 55-305).
Ref:	=2001ApJ...562L..35V
by	VAN DOKKUM P.G. , STANFORD S.A.
	Astrophys. J., 562, 35-38 (2001)
	A massive disk galaxy at z=1.34.
o	L451 in the Lynx field = EES 451 in SIMBAD. RDCS J0848+4453 = ClG J0848+4453
o	<EES NNN> (No. 451) added. <RDCS J0848+4453> N=1.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EES2006]
[EES2006]	(Einasto+Einasto+Saar+, 2006)
Write:	<<[EES2006] NNN>>
N:	911
Object:	Supercluster of G (SIMBAD class: SuperClG = Supercluster of Galaxies)
Note:	Compilation of a supercluster sample using SDSS DR4.
Ref:	=2006A&A...459L...1E
by	EINASTO J. , EINASTO M., SAAR E., TAGO E., LIIVAMAEGI L.J., JOEVEER M., SUHHONENKO I., HUETSI G., JAANISTE J., HEINAEMAEKI P., MUELLER V., KNEBE A., TUCKER D.
	Astron. Astrophys., 459L, 1-4 (2006)
	Luminous superclusters: remnants from inflation?
o	Tables 4a, 4b: <[EES2006] NNN> (Nos 1-911).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EES2009]
[EES2009]	(Enoch+Evans+Sargent+, 2009)
Write:	<<[EES2009] Per-emb NN>> <<[EES2009] Ser-emb NN>> <<[EES2009] Oph-emb NN>>
N:	66+34+28
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	Caltech Submillimeter Observatory Bolocam 1.1mm continuum and Spitzer Legacy surveys of the Perseus, Serpens, Ophiuchus molecular clouds.
in source:	NAME Perseus Molecular Cloud
in source:	NAME Serpens Cloud
in source:	NAME rho Oph Cloud
Ref:	=2009ApJ...692..973E
by	ENOCH M.L. , EVANS N.J., SARGENT A.I., GLENN J.
	Astrophys. J., 692, 973-997 (2009)
	Properties of the youngest protostars in Perseus, Serpens, and Ophiuchus.
o	Tables 2-4: <[EES2009] Per-emb NN> (Nos 1-66), <[EES2009] Ser-emb NN> (Nos 1-34), <[EES2009] Oph-emb NN> (Nos 1-28).
=E=	Catalogue in electronic form as <J/ApJ/692/973/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EES2012]
[EES2012]	(Elmegreen+Elmegreen+Sanchez Almeida+, 2012)
Write:	<<[EES2012] Kiso NNNN>>
N:	13+36
Object:	G (SIMBAD class: Galaxy)
Note:	Kiso Schmidt telescope observations within the Kiso survey for Ultraviolet-Excess Galaxies.
Ref:	=2012ApJ...750...95E
by	ELMEGREEN D.M. , ELMEGREEN B.G., SANCHEZ ALMEIDA J., MUNOZ-TUNON C., PUTKO J., DEWBERRY J.
	Astrophys. J., 750, 95 (2012)
	Local tadpole galaxies.
o	Table 1: <[EES2012] Kiso NNNN> N=13 among (Nos 3193 to 8466).
Ref:	=2013ApJ...774...86E
by	ELMEGREEN B.G. , ELMEGREEN D.M., SANCHEZ ALMEIDA J., MUNOZ-TUNON C., DEWBERRY J., PUTKO J., TEICH Y., POPINCHALK M.
	Astrophys. J., 774, 86 (2013)
	Massive clumps in local galaxies: comparisons with high-redshift clumps.
o	Table 1: <[EES2012] Kiso NNNN> N=36 among (Nos 2205-9363).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EET2007]
[EET2007]	(Einasto+Einasto+Tago+, 2007)= (2dF) = (2dFGRS)
Write:	<<[EET2007] NNNN>> <<[EET2007] SNNN>>
N:	229+314
Object:	Supercluster of G (SIMBAD class: SuperClG = Supercluster of Galaxies)
Note:	2dF Galaxy Redshift Survey data are used to compile catalogues of superclusters for the Northern and Southern regions of the 2dFGRS.
Ref:	=2007A&A...462..811E
by	EINASTO J. , EINASTO M., TAGO E., SAAR E., HUETSI G., JOEVEER M., LIIVAMAEGI L.J., SUHHONENKO I., JAANISTE J., HEINAEMAEKI P., MUELLER V., KNEBE A., TUCKER D.
	Astron. Astrophys., 462, 811-825 (2007)
	Superclusters of galaxies from the 2dF redshift survey. I. The catalogue.
o	Catalogues: <[EET2007] WNNN> (Nos N1-N229, S1-S314).
=E=	Catalogue in electronic form as J/A+A/462/811
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EET94]
[EET94]	(Einasto+Einasto+Tago+, 1994)= (SC)
Write:	<<[EET94] SCG NNN>> <<[EET94] Void NN>>
N:	130+27
Object:	Supercluster of G + Void (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=130 superclusters of G, format 'SCG NNN'. See also SCl. Table 5: N=27 voids, format 'Void NN'. See also [BB85], [S2000h].
Ref:	=1994MNRAS.269..301E
by	EINASTO M. , EINASTO J., TAGO E., DALTON G.B., ANDERNACH H.
	Mon. Not. R. Astron. Soc., 269, 301-322 (1994)
	The structure of the universe traced by rich clusters of galaxies.
o	In 1997A&AS..123..119E, Einasto+ say: Some superclusters were misordered in Table 3 of 1994MNRAS.269..301E. They use Table 2 of 1994MNRAS.269..301E for cross-identifications in Table A1 of 1997A&AS..123..119E.
o	Table 2: <[EET94] SCG NNN> N=130. Table 5: <[EET94] Void NN> N=27
=E=	Catalogue in electronic form as J/MNRAS/269/301
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EF
EF	(Effelsberg)
Write:	<<EF BHHMM+DDMM>>
N:	234
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1994A&AS..106..303N
by	NEUMANN M. , REICH W., FUERST E., BRINKMANN W., REICH P., SIEBERT J., WIELEBINSKI R., TRUEMPER J.
	Astron. Astrophys., Suppl. Ser., 106, 303-326 (1994)
	Multifrequency observations of ROSAT selected radio sources.
o	Table 2: <EF BHHMM+DDMM> N=234
=E=	Catalogue in electronic form as J/A+AS/106/303
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EF
EF	(Elias+Frogel)
*****	Avoid the usage of EF, prefer [EF85]
Origin	of the Acronym: L (1999A&A...346...33A)
Details on Acronym: [EF2003]
[EF2003]	(English+Freeman, 2003)
Write:	<<[EF2003] BN>>
N:	7
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	See also paper II: [ENF2003].
in source:	NGC 3256
Ref:	=2003AJ....125.1124E
by	ENGLISH J. , FREEMAN K.C.
	Astron. J., 125, 1124-1133 (2003)
	Giant H II regions in the merging system NGC 3256: are they the birthplaces of globular clusters.
o	Fig.2: Stars A, B, C not in SIMBAD.
o	Fig.1, Table 1: <[EF2003] BN> (Nos B1-B7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EF2011]
[EF2011]	(Edwards+Fadda, 2011)
Write:	<<[EF2011] NNNN>>
N:	7608
Object:	(MIR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Palomar 200" telescope WIRC NIR and Spitzer MIPS MIR observations of the Coma cluster of galaxies.
in source:	Coma Cluster = ACO 1656
Ref:	=2011AJ....142..148E
by	EDWARDS L.O.V. , FADDA D.
	Astron. J., 142, 148 (2011)
	A multi-wavelength analysis of Spitzer selected Coma cluster galaxies: star formation rates and masses.
o	(Erratum) erratum vol. 143, art. 151 (2012)
o	Table 3: <[EF2011] NNNN> (Nos 1-7608).
=E=	Catalogue in electronic form as J/AJ/142/148
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EF85]
[EF85]	(Elias+Frogel, 1985)= (EF)
Write:	<<[EF85] NGC 3109 NN>> <<[EF85] DDO 210 N>>
N:	16+8
Object:	M supergiant (SIMBAD class: Star)
in source:	NGC 3109
in source:	NAME Aquarius Dwarf Galaxy = DDO 210
Ref:	=1985ApJ...289..141E
by	ELIAS J.H. , FROGEL J.A.
	Astrophys. J., 289, 141-149 (1985)
	M supergiants in local group irregular galaxies : metallicities and distances.
o	T.2: SMC Case NNN-NN = [S84d] NNN-NN
o	Table 3, Fig.1: <[EF85] NGC 3109 NN> (Nos 1-16). Table 3, Fig.2: <[EF85] DDO 210 N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EFAR
EFAR	(EFAR system)
*****	Avoid the usage of EFAR, prefer [WCB96]
Origin	of the Acronym: L (1997MNRAS.287..899L)
Details on Acronym: [EFB2010]
[EFB2010]	(Erlund+Fabian+Blundell+, 2010)= ([EFB2010a])
Write:	<<[EFB2010] peak>> <<[EFB2010] southern arc>> <<[EFB2010] jet knot>>
N:	1+1+1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra X-ray observations of the quasar 4C 74.26.
in source:	4C 74.26
Ref:	=2010MNRAS.404..629E
by	ERLUND M.C. , FABIAN A.C., BLUNDELL K.M., CRAWFORD C.S., HIRST P.
	Mon. Not. R. Astron. Soc., 404, 629-640 (2010)
	Two types of shock in the hotspot of the giant quasar 4C74.26: a high-resolution comparison from Chandra, Gemini and MERLIN.
o	Text: <[EFB2010] peak> N=1, <[EFB2010] southern arc> N=1, <[EFB2010] jet knot> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EFB2010a]
[EFB2010a]	(Erlund+Fabian+Blundell+, 2010)
Note:	Chandra, Gemini and WHT observations of the quasar 4C 74.26.
*****	Avoid the usage of [EFB2010a], prefer [EFB2010]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EFB2010b]
[EFB2010b]	(Edwards+Fadda+Biviano+, 2010)
Write:	<<[EFB2010b] MIPS24 NNNNN>> <<[EFB2010b] MIPS70 NNNN>>
N:	10876+1545
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Spitzer MIPS (24 and 70mu.m) and Palomar 200in rJHK observations of ACO 1763.
in source:	ACO 1763
Ref:	=2010AJ....139..434E
by	EDWARDS L.O.V. , FADDA D., BIVIANO A., MARLEAU F.R.
	Astron. J., 139, 434-446 (2010)
	Spitzer observations of Abell 1763. I. Infrared and optical photometry.
o	Table 2: <[EFB2010b] MIPS24 NNNNN> (Nos 1-10876). Table 3: <[EFB2010b] MIPS70 NNNN> N=733 among (Nos 1-1545).
=E=	Catalogue in electronic form as <J/AJ/139/434/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EFE2001]
[EFE2001]	(Eikenberry+Fischer+Egami+, 2001)
Write:	<<[EFE2001] 1758-258 A>> <<[EFE2001] 1740-2942 A>> <<[EFE2001] 1758-258 a>>
N:	5+3+2
Object:	* (SIMBAD class: Star)
Note:	Keck observations. Fig.1: (Nos A-E), 5 calibration stars in the field of GRANAT 1758-258. Fig.2: (Nos A-C), 3 calibration stars in the field of 1E 1740.7-2942. Fig.4, Table 2: sources inside the error box of GRANAT 1758-258, star A already in Fig.1 and (Nos b-c). In Fig.3 and Table 1: [MMC2000] objects.
Ref:	=2001ApJ...556....1E
by	EIKENBERRY S.S. , FISCHER W.J., EGAMI E., DJORGOVSKI S.G.
	Astrophys. J., 556, 1-5 (2001)
	Deep infrared imaging of the microquasars 1E 1740-2942 and GRS 1758-258.
o	Fig.1: <[EFE2001] 1758-258 A> (Nos A-E). Fig.2: <[EFE2001] 1740-2942 A> (Nos A-C). Fig.3: <[EFE2001] 1758-258 a> (Nos b-c).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: eFEDS
eFEDS	(eROSITA Final Equatorial-Depth Survey)
Write:	<<eFEDS JHHMMSS.s+DDMMSS>>
N:	about 33000
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	In November 2019, eROSITA on board of the Spektrum-Roentgen-Gamma (SRG) observatory started to map the entire sky in X-rays. After the four-year survey program, it will reach a flux limit that is about 25 times deeper than ROSAT. During the SRG performance verification phase, eROSITA (https://erosita.mpe.mpg.de) observed a contiguous 140 deg2 area of the sky down to the final depth of the eROSITA all-sky survey (eROSITA Final Equatorial- Depth Survey; eFEDS), with the goal of obtaining a census of the X-ray emitting populations (stars, compact objects, galaxies, clusters of galaxies, and active galactic nuclei) that will be discovered over the entire sky. The name registered here is for eFEDS.
Notes:	Already about 45 papers part of an A&A special issue on the eROSITA early data release on the eFEDS field make use of this nomenclature. More will come from the eROSITA collaboration and from the entire astronomy community.
Ref:	=2022A&A...661A...1B
by	BRUNNER H. , LIU T., LAMER G., GEORGAKAKIS A., MERLONI A., BRUSA M., BULBUL E., DENNERL K., FRIEDRICH S., LIU A., MAITRA C., NANDRA K., RAMOS-CEJA M.E., SANDERS J.S., STEWART I.M., BOLLER T., BUCHNER J., CLERC N., COMPARAT J., DWELLY T., ECKERT D., FINOGUENOV A., FREYBERG M., GHIRARDINI V., GUEGUEN A., HABERL F., KREYKENBOHM I., KRUMPE M., OSTERHAGE S., PACAUD F., PREDEHL P., REIPRICH T.H., ROBRADE J., SALVATO M., SANTANGELO A., SCHRABBACK T., SCHWOPE A., WILMS J.
	Astron. Astrophys., 661A, 1-1 (2022)
	The eROSITA Final Equatorial Depth Survey (eFEDS). X-ray catalogue.
o	<eFEDS JHHMMSS.s+DDMMSS> N=27910+4774. MPE
=E=	Catalogue in electronic form as <J/A+A/661/A1/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: eFEDS-SC
eFEDS-SC	(eROSITA Final Equatorial-Depth Survey - Supercluster Candidate)
Write:	<<eFEDS-SC NN>>
N:	19
Object:	Poss. Supercluster of G (SIMBAD class: SuperClG_Candidate = Supercluster of Galaxies Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=19 supercluster candidates in the eFEDS field, as part of the eROSITA Final Equatorial-Depth Survey.
Ref:	=2022A&A...661A...2L
by	LIU A. , BULBUL E., GHIRARDINI V., LIU T., KLEIN M., CLERC N., OZSOY Y., RAMOS-CEJA M.E., PACAUD F., COMPARAT J., OKABE N., BAHAR Y.E., BIFFI V., BRUNNER H., BRUGGEN M., BUCHNER J., IDER CHITHAM J., CHIU I., DOLAG K., GATUZZ E., GONZALEZ J., HOANG D.N., LAMER G., MERLONI A., NANDRA K., OGURI M., OTA N., PREDEHL P., REIPRICH T.H., SALVATO M., SCHRABBACK T., SANDERS J.S., SEPPI R., THIBAUD Q.
	Astron. Astrophys., 661A, 2-2 (2022)
	The eROSITA Final Equatorial-Depth Survey (eFEDS). Catalog of galaxy clusters and groups.
o	Fig. A.1, Tables 4+A.1: <eFEDS-SCNN> (Nos SC1-SC19).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EFF2010]
[EFF2010]	(Edwards+Fadda+Frayer+, 2010)
Write:	<<[EFF2010] DDD.dddddd+DD.dddddd>> <<[EFF2010] AN>>
N:	29+33+11
Object:	(Rad) + (X) + G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLA observations of ACO 1763 and use of XMM-Newton archive. In the format AN: cluster core members are labeled "C", those in the filament "F", and those with absorption line spectra "A".
in source:	ACO 1763
Ref:	=2010AJ....140.1891E
by	EDWARDS L.O.V. , FADDA D., FRAYER D.T., LIMA NETO G.B., DURRET F.
	Astron. J., 140, 1891-1904 (2010)
	Spitzer observations of A1763. II. Constraining the nature of activity in the cluster-feeding filament with VLA and XMM-Newton data.
o	Tables 2-3: <[EFF2010] DDD.dddddd+DD.dddddd> N=29+33. Table 2: <[EFF2010] AN> (Nos A1-A3, C1-C2, F1-F6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Effelsberg
Effelsberg	(Effelsberg survey)
*****	Avoid the usage of Effelsberg, prefer RFS
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [EFG2005]
[EFG2005]	(Edris+Fuller+Cohen+, 2005) (Not yet in Simbad)
Write:	<<[EFG2005] OH JHHMMSS.sss+DDMMSS.ss>> <<[EFG2005] H2O JHHMMSS.sss+DDMMSS.sss>> <<[EFG2005] CH3OH JHHMMSS.sss+DDMMSS.sss>> <<[EFG2005] OH JHHMMSS.ssss+DDMMSS.sss>> <<[EFG2005] OH RN>> <<[EFG2005] OH LN>> <<[EFG2005] OH N>> <<[EFG2005] H2O JHHMMSS.ssss+DDMMSS.sss>> <<[EFG2005] H2O N>>
N:	1+1+1+9+8
Object:	Maser (SIMBAD class: Maser)
Note:	MERLIN observations of masers towards IRAS 20126+4104. Table 2: brightest maser spots in OH, H2O, CH3OH. Tables 3, 4: N=9 OH maser components, with Right or Left polarization. Table 5: N=7 H2O maser components.
Ref:	=2005A&A...434..213E
by	EDRIS K.A. , FULLER G.A., COHEN R.J., ETOKA S.
	Astron. Astrophys., 434, 213-220 (2005)
	The masers towards IRAS 20126+4104.
o	Table 2: <[EFG2005] OH JHHMMSS.sss+DDMMSS.ss> N=1, <[EFG2005] H2O JHHMMSS.sss+DDMMSS.ss> N=1, <[EFG2005] CH3OH JHHMMSS.sss+DDMMSS.ss> N=1. Table 3: <[EFG2005] OH JHHMMSS.ssss+DDMMSS.sss> N=7+2, <[EFG2005] OH RN> (Nos R1-R7), <[EFG2005] OH LN> (Nos L1-L2). Table 4: <[EFG2005] OH N> (Nos 1-9). Table 5: <[EFG2005] H2O JHHMMSS.ssss+DDMMSS.sss> N=8 = <[EFG2005] H2O N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EFG2012]
[EFG2012]	(Evans+Fridriksson+Gehrels+, 2012)
Write:	<<[EFG2012] {J\|S\|V}NN>>
N:	8+12+11
Object:	(X) + V* (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Swift XRT and UVOT observations of N=8+12 detections in the fields of two candidate gravitational-wave transient events (respectively in January - leading J in the format - and in September - leading S in the format). N=11 potential variable stars were also detected in the Swift UVOT data.
Ref:	=2012ApJS..203...28E
by	EVANS P.A. , FRIDRIKSSON J.K., GEHRELS N., HOMAN J., OSBORNE J.P., SIEGEL M., BEARDMORE A., HANDBAUER P., GELBORD J., KENNEA J.A., SMITH M., ZHU Q., (The LIGO Scientific Collaboration), (The Virgo Collaboration), AASI J., ABADIE J., ABBOTT B.P., ABBOTT R., ABBOTT T.D., ABERNATHY M., ACCADIA T., ACERNESE F., ADAMS C., ADAMS T., ADDESSO P., ADHIKARI R., AFFELDT C., AGATHOS M., AGATSUMA K., AJITH P., ALLEN B., ALLOCCA A., AMADOR CERON E., AMARIUTEI D., ANDERSON S.B., ANDERSON W.G., ARAI K., ARAYA M.C., AST S., ASTON S.M., ASTONE P., ATKINSON D., AUFMUTH P., AULBERT C., AYLOTT B.E., BABAK S., BAKER P., BALLARDIN G., BALLMER S., BAO Y., BARAYOGA J.C.B., BARKER D., BARONE F., BARR B., BARSOTTI L., BARSUGLIA M., BARTON M.A., BARTOS I., BASSIRI R., BASTARRIKA M., BASTI A., BATCH J., BAUCHROWITZ J., BAUER Th.S., BEBRONNE M., BECK D., BEHNKE B., BEJGER M., BEKER M.G., BELL A.S., BELL C., BELOPOLSKI I., BENACQUISTA M., BERLINER J.M., BERTOLINI A., BETZWIESER J., BEVERIDGE N., BEYERSDORF P.T., BHADBADE T., BILENKO I.A., BILLINGSLEY G., BIRCH J., BISWAS R., BITOSSI M., BIZOUARD M.A., BLACK E., BLACKBURN J.K., BLACKBURN L., BLAIR D., BLAND B., BLOM M., BOCK O., BODIYA T.P., BOGAN C., BOND C., BONDARESCU R., BONDU F., BONELLI L., BONNAND R., BORK R., BORN M., BOSCHI V., BOSE S., BOSI L., BOUHOU B., BRACCINI S., BRADASCHIA C., BRADY P.R., BRAGINSKY V.B., BRANCHESI M., BRAU J.E., BREYER J., BRIANT T., BRIDGES D.O., BRILLET A., BRINKMANN M., BRISSON V., BRITZGER M., BROOKS A.F., BROWN D.A., BULIK T., BULTEN H.J., BUONANNO A., BURGUET-CASTELL J., BUSKULIC D., BUY C., BYER R.L., CADONATI L., CAGNOLI G., CALLONI E., CAMP J.B., CAMPSIE P., CANNON K., CANUEL B., CAO J., CAPANO C.D., CARBOGNANI F., CARBONE L., CARIDE S., CAUDILL S., CAVAGLIA M., CAVALIER F., CAVALIERI R., CELLA G., CEPEDA C., CESARINI E., CHALERMSONGSAK T., CHARLTON P., CHASSANDE-MOTTIN E., CHEN W., CHEN X., CHEN Y., CHINCARINI A., CHIUMMO A., CHO H.S., CHOW J., CHRISTENSEN N., CHUA S.S.Y., CHUNG C.T.Y., CHUNG S., CIANI G., CLARA F., CLARK D.E., CLARK J.A., CLAYTON J.H., CLEVA F., COCCIA E., COHADON P.-F., COLACINO C.N., COLLA A., COLOMBINI M., CONTE A., CONTE R., COOK D., CORBITT T.R., CORDIER M., CORNISH N., CORSI A., COSTA C.A., COUGHLIN M., COULON J.-P., COUVARES P., COWARD D.M., COWART M., COYNE D.C., CREIGHTON J.D.E., CREIGHTON T.D., CRUISE A.M., CUMMING A., CUNNINGHAM L., CUOCO E., CUTLER R.M., DAHL K., DAMJANIC M., DANILISHIN S.L., D'ANTONIO S., DANZMANN K., DATTILO V., DAUDERT B., DAVELOZA H., DAVIER M., DAW E.J., DAY R., DAYANGA T., DE ROSA R., DEBRA D., DEBRECZENI G., DEGALLAIX J., DEL POZZO W., DENT T., DERGACHEV V., DEROSA R., DHURANDHAR S., DI FIORE L., DI LIETO A., DI PALMA I., DI PAOLO EMILIO M., DI VIRGILIO A., DIAZ M., DIETZ A., DONOVAN F., DOOLEY K.L., DORAVARI S., DORSHER S., DRAGO M., DREVER R.W.P., DRIGGERS J.C., DU Z., DUMAS J.-C., DWYER S., EBERLE T., EDGAR M., EDWARDS M., EFFLER A., EHRENS P., EIKENBERRY S., ENDROCZI G., ENGEL R., ETZEL T., EVANS K., EVANS M., EVANS T., FACTOUROVICH M., FAFONE V., FAIRHURST S., FARR B.F., FAVATA M., FAZI D., FEHRMANN H., FELDBAUM D., FERRANTE I., FERRINI F., FIDECARO F., FINN L.S., FIORI I., FISHER R.P., FLAMINIO R., FOLEY S., FORSI E., FORTE L.A., FOTOPOULOS N., FOURNIER J.-D., FRANC J., FRANCO S., FRASCA S., FRASCONI F., FREDE M., FREI M.A., FREI Z., FREISE A., FREY R., FRICKE T.T., FRIEDRICH D., FRITSCHEL P., FROLOV V.V., FUJIMOTO M.-K., FULDA P.J., FYFFE M., GAIR J., GALIMBERTI M., GAMMAITONI L., GARCIA J., GARUFI F., GASPAR M.E., GELENCSER G., GEMME G., GENIN E., GENNAI A., GERGELY L.A., GHOSH S., GIAIME J.A., GIAMPANIS S., GIARDINA K.D., GIAZOTTO A., GIL-CASANOVA S., GILL C., GLEASON J., GOETZ E., GONZALEZ G., GORODETSKY M.L., GOSSLER S., GOUATY R., GRAEF C., GRAFF P.B., GRANATA M., GRANT A., GRAY C., GREENHALGH R.J.S., GRETARSSON A.M., GRIFFO C., GROTE H., GROVER K., GRUNEWALD S., GUIDI G.M., GUIDO C., GUPTA R., GUSTAFSON E.K., GUSTAFSON R., HALLAM J.M., HAMMER D., HAMMOND G., HANKS J., HANNA C., HANSON J., HARMS J., HARRY G.M., HARRY I.W., HARSTAD E.D., HARTMAN M.T., HAUGHIAN K., HAYAMA K., HAYAU J.-F., HEEFNER J., HEIDMANN A., HEINTZE M.C., HEITMANN H., HELLO P., HEMMING G., HENDRY M.A., HENG I.S., HEPTONSTALL A.W., HERRERA V., HEURS M., HEWITSON M., HILD S., HOAK D., HODGE K.A., HOLT K., HOLTROP M., HONG T., HOOPER S., HOUGH J., HOWELL E.J., HUGHEY B., HUSA S., HUTTNER S.H., HUYNH-DINH T., INGRAM D.R., INTA R., ISOGAI T., IVANOV A., IZUMI K., JACOBSON M., JAMES E., JANG Y.J., JARANOWSKI P., JESSE E., JOHNSON W.W., JONES D.I., JONES R., JONKER R.J.G., JU L., KALMUS P., KALOGERA V., KANDHASAMY S., KANG G., KANNER J.B., KASPRZACK M., KASTURI R., KATSAVOUNIDIS E., KATZMAN W., KAUFER H., KAUFMAN K., KAWABE K., KAWAMURA S., KAWAZOE F., KEITEL D., KELLEY D., KELLS W., KEPPEL D.G., KERESZTES Z., KHALAIDOVSKI A., KHALILI F.Y., KHAZANOV E.A., KIM B.K., KIM C., KIM H., KIM K., KIM N., KIM Y.M., KING P.J., KINZEL D.L., KISSEL J.S., KLIMENKO S., KLINE J., KOKEYAMA K., KONDRASHOV V., KORANDA S., KORTH W.Z., KOWALSKA I., KOZAK D., KRINGEL V., KRISHNAN B., KROLAK A., KUEHN G., KUMAR P., KUMAR R., KURDYUMOV R., KWEE P., LAM P.K., LANDRY M., LANGLEY A., LANTZ B., LASTZKA N., LAWRIE C., LAZZARINI A., LE ROUX A., LEACI P., LEE C.H., LEE H.K., LEE H.M., LEONG J.R., LEONOR I., LEROY N., LETENDRE N., LHUILLIER V., LI J., LI T.G.F., LINDQUIST P.E., LITVINE V., LIU Y., LIU Z., LOCKERBIE N.A., LODHIA D., LOGUE J., LORENZINI M., LORIETTE V., LORMAND M., LOSURDO G., LOUGH J., LUBINSKI M., LUCK H., LUNDGREN A.P., MacARTHUR J., MacDONALD E., MACHENSCHALK B., MACINNIS M., MacLEOD D.M., MAGESWARAN M., MAILAND K., MAJORANA E., MAKSIMOVIC I., MALVEZZI V., MAN N., MANDEL I., MANDIC V., MANTOVANI M., MARCHESONI F., MARION F., MARKA S., MARKA Z., MARKOSYAN A., MAROS E., MARQUE J., MARTELLI F., MARTIN I.W., MARTIN R.M., MARX J.N., MASON K., MASSEROT A., MATICHARD F., MATONE L., MATZNER R.A., MAVALVALA N., MAZZOLO G., McCARTHY R., McCLELLAND D.E., McDANIEL P., McGUIRE S.C., McINTYRE G., McIVER J., MEADORS G.D., MEHMET M., MEIER T., MELATOS A., MELISSINOS A.C., MENDELL G., MENENDEZ D.F., MERCER R.A., MESHKOV S., MESSENGER C., MEYER M.S., MIAO H., MICHEL C., MILANO L., MILLER J., MINENKOV Y., MINGARELLI C.M.F., MITROFANOV V.P., MITSELMAKHER G., MITTLEMAN R., MOE B., MOHAN M., MOHAPATRA S.R.P., MORARU D., MORENO G., MORGADO N., MORGIA A., MORI T., MORRISS S.R., MOSCA S., MOSSAVI K., MOURS B., MOW-LOWRY C.M., MUELLER C.L., MUELLER G., MUKHERJEE S., MULLAVEY A., MULLER-EBHARDT H., MUNCH J., MURPHY D., MURRAY P.G., MYTIDIS A., NASH T., NATICCHIONI L., NECULA V., NELSON J., NERI I., NEWTON G., NGUYEN T., NISHIZAWA A., NITZ A., NOCERA F., NOLTING D., NORMANDIN M.E., NUTTALL L., OCHSNER E., O'DELL J., OELKER E., OGIN G.H., OH J.J., OH S.H., OLDENBERG R.G., O'REILLY B., O'SHAUGHNESSY R., OSTHELDER C., OTT C.D., OTTAWAY D.J., OTTENS R.S., OVERMIER H., OWEN B.J., PAGE A., PALLADINO L., PALOMBA C., PAN Y., PANKOW C., PAOLETTI F., PAOLETTI R., PAPA M.A., PARISI M., PASQUALETTI A., PASSAQUIETI R., PASSUELLO D., PEDRAZA M., PENN S., PERRECA A., PERSICHETTI G., PHELPS M., PICHOT M., PICKENPACK M., PIERGIOVANNI F., PIERRO V., PIHLAJA M., PINARD L., PINTO I.M., PITKIN M., PLETSCH H.J., PLISSI M.V., POGGIANI R., POLD J., POSTIGLIONE F., POUX C., PRATO M., PREDOI V., PRESTEGARD T., PRICE L.R., PRIJATELJ M., PRINCIPE M., PRIVITERA S., PRIX R., PRODI G.A., PROKHOROV L.G., PUNCKEN O., PUNTURO M., PUPPO P., QUETSCHKE V., QUITZOW-JAMES R., RAAB F.J., RABELING D.S., RACZ I., RADKINS H., RAFFAI P., RAKHMANOV M., RAMET C., RANKINS B., RAPAGNANI P., RAYMOND V., RE V., REED C.M., REED T., REGIMBAU T., REID S., REITZE D.H., RICCI F., RIESEN R., RILES K., ROBERTS M., ROBERTSON N.A., ROBINET F., ROBINSON C., ROBINSON E.L., ROCCHI A., RODDY S., RODRIGUEZ C., RODRUCK M., ROLLAND L., ROLLINS J.G., ROMANO J.D., ROMANO R., ROMIE J.H., ROSINSKA D., ROVER C., ROWAN S., RUDIGER A., RUGGI P., RYAN K., SALEMI F., SAMMUT L., SANDBERG V., SANKAR S., SANNIBALE V., SANTAMARIA L., SANTIAGO-PRIETO I., SANTOSTASI G., SARACCO E., SASSOLAS B., SATHYAPRAKASH B.S., SAULSON P.R., SAVAGE R.L., SCHILLING R., SCHNABEL R., SCHOFIELD R.M.S., SCHULZ B., SCHUTZ B.F., SCHWINBERG P., SCOTT J., SCOTT S.M., SEIFERT F., SELLERS D., SENTENAC D., SERGEEV A., SHADDOCK D.A., SHALTEV M., SHAPIRO B., SHAWHAN P., SHOEMAKER D.H., SIDERY T.L., SIEMENS X., SIGG D., SIMAKOV D., SINGER A., SINGER L., SINTES A.M., SKELTON G.R., SLAGMOLEN B.J.J., SLUTSKY J., SMITH J.R., SMITH M.R., SMITH R.J.E., SMITH-LEFEBVRE N.D., SOMIYA K., SORAZU B., SPEIRITS F.C., SPERANDIO L., STEFSZKY M., STEINERT E., STEINLECHNER J., STEINLECHNER S., STEPLEWSKI S., STOCHINO A., STONE R., STRAIN K.A., STRIGIN S.E., STROEER A.S., STURANI R., STUVER A.L., SUMMERSCALES T.Z., SUNG M., SUSMITHAN S., SUTTON P.J., SWINKELS B., SZEIFERT G., TACCA M., TAFFARELLO L., TALUKDER D., TANNER D.B., TARABRIN S.P., TAYLOR R., TER BRAACK A.P.M., THOMAS P., THORNE K.A., THORNE K.S., THRANE E., THURING A., TITSLER C., TOKMAKOV K.V., TOMLINSON C., TONCELLI A., TONELLI M., TORRE O., TORRES C.V., TORRIE C.I., TOURNEFIER E., TRAVASSO F., TRAYLOR G., TSE M., UGOLINI D., VAHLBRUCH H., VAJENTE G., VAN DEN BRAND J.F.J., VAN DEN BROECK C., VAN DER PUTTEN S., VAN VEGGEL A.A., VASS S., VASUTH M., VAULIN R., VAVOULIDIS M., VECCHIO A., VEDOVATO G., VEITCH J., VEITCH P.J., VENKATESWARA K., VERKINDT D., VETRANO F., VICERE A., VILLAR A.E., VINET J.-Y., VITALE S., VOCCA H., VORVICK C., VYATCHANIN S.P., WADE A., WADE L., WADE M., WALDMAN S.J., WALLACE L., WAN Y., WANG M., WANG X., WANNER A., WARD R.L., WAS M., WEINERT M., WEINSTEIN A.J., WEISS R., WELBORN T., WEN L., WESSELS P., WEST M., WESTPHAL T., WETTE K., WHELAN J.T., WHITCOMB S.E., WHITE D.J., WHITING B.F., WIESNER K., WILKINSON C., WILLEMS P.A., WILLIAMS L., WILLIAMS R., WILLKE B., WIMMER M., WINKELMANN L., WINKLER W., WIPF C.C., WISEMAN A.G., WITTEL H., WOAN G., WOOLEY R., WORDEN J., YABLON J., YAKUSHIN I., YAMAMOTO H., YAMAMOTO K., YANCEY C.C., YANG H., YEATON-MASSEY D., YOSHIDA S., YVERT M., ZADROZNY A., ZANOLIN M., ZENDRI J.-P., ZHANG F., ZHANG L., ZHAO C., ZOTOV N., ZUCKER M.E., ZWEIZIG J.
	Astrophys. J., Suppl. Ser., 203, 28 (2012)
	Swift follow-up observations of candidate gravitational-wave transient events.
o	Tables 3+5: <[EFG2012] JN> (Nos 1-8). Tables 4+6: <[EFG2012] SNN> (Nos 1-12). Table 7: <[EFG2012] VNN> (Nos V1-V11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EFH2009]
[EFH2009]	(Eliasdotir+Fynbo+Hjorth+, 2009)
Write:	<<[EFH2009] GRB 070802 host G>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ESO VLT observations of GRB 070802 host galaxy.
Ref:	=2009ApJ...697.1725E
by	ELIASDOTTIR A. , FYNBO J.P.U., HJORTH J., LEDOUX C., WATSON D.J., ANDERSEN A.C., MALESANI D., VREESWIJK P.M., PROCHASKA J.X., SOLLERMAN J., JAUNSEN A.O.
	Astrophys. J., 697, 1725-1740 (2009)
	Dust extinction in high-z galaxies with γ-ray burst afterglow spectroscopy: the 2175 Å feature at z = 2.45.
o	Paragr. 2.3: <[EFH2009] GRB 070802 host G> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EFK91]
[EFK91]	(Evans+Ford+Kinney+, 1991)
Write:	<<[EFK91] A>>
N:	9
Object:	Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	HST PC observations. See also [DW98]
in source:	NGC 1068
Ref:	=1991ApJ...369L..27E
by	EVANS I.N. , FORD H.C., KINNEY A.L., ANTONUCCI R.R.J., ARMUS L., CAGANOFF S.
	Astrophys. J., 369, 27-30 (1991)
	HST imaging of the inner 3 arcseconds of NGC 1068 in the light of O III λ 5007.
o	<[EFK91] A> (Nos A-G)
Ref:	=2000ApJ...532..247C
by	CRENSHAW D.M. , KRAEMER S.B.
	Astrophys. J., 532, 247-255 (2000)
	Resolved spectroscopy of the narrow-line region in NGC 1068. I. The nature of the continuum emission.
o	Fig.1: <[EFK91] A> (Nos H-I) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EFR
EFR	(EFAR system)
*****	Avoid the usage of EFR, prefer [WCB96]
Origin	of the Acronym: L (2000MNRAS.313..469S)
Details on Acronym: [EFS2003]
[EFS2003]	(Eisloffel+Froebrich+Stanke+, 2003)
Write:	<<[EFS2003] N-a>>
N:	43
Object:	H2 e. knot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Calar Alto 3.5m telescope NIR wide field survey of the open star cluster IC 348. H2 emission knots in 5 regions around IC 348.
in source:	IC 348
Ref:	=2003ApJ...595..259E
by	EISLOEFFEL J. , FROEBRICH D., STANKE T., McCAUGHREAN M.J.
	Astrophys. J., 595, 259-265 (2003)
	Molecular outflows in the young open cluster IC 348.
o	<NAME IC 348 MMS> N=1. Table 1: <[EFS2003] N-a> (Nos 1-a to 1-w, 2-a to 2-h, 3-a to 3-f, 4-a to 4-b, 5-a to 5-d).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EFT2013]
[EFT2013]	(Erfanianfar+Finoguenov+Tanaka+, 2013)
Write:	<<[EFT2013] DDD.dddddd+DD.dddddd>> <<[EFT2013] JHHMM.m+DDMM>>
N:	52+387
Object:	Group of G + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	DEEP2/DEEP3 Keck DEIMOS and MMT Hectospec observations of N=387 extended X-ray sources and their N=52 corresponding galaxy groups in the Extended Groth Strip (EGS).
in source:	NAME Extended Groth Strip
Ref:	=2013ApJ...765..117E
by	ERFANIANFAR G. , FINOGUENOV A., TANAKA M., LERCHSTER M., NANDRA K., LAIRD E., CONNELLY J.L., BIELBY R., MIRKAZEMI M., FABER S.M., KOCEVSKI D., COOPER M., NEWMAN J.A., JELTEMA T., COIL A.L., BRIMIOULLE F., DAVIS M., McCRACKEN H.J., WILLMER C., GERKE B., CAPPELLUTI N., GWYN S.
	Astrophys. J., 765, 117 (2013)
	X-ray groups of galaxies in the AEGIS deep and wide fields.
o	Table 1: <[EFT2013] JHHMM.m+DDMM> N=52. Table 2: <[EFT2013] DDD.dddddd+DD.dddddd> N=387.
=E=	Catalogue in electronic form as <J/ApJ/765/117/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EG
EG	(Eggen+Greenstein)
Rem:	(Nos 1-266)
*****	Avoid the usage of EG, prefer EGGR
Details on Acronym: EG B
EG B	(Ellis+Grayson+Bond) (Not yet in Simbad)
*****	Avoid the usage of EG B, prefer EGB
Origin	of the Acronym: L = Found in the literature
Details on Acronym: 1EG
1EG	(1st EGRET Gamma-ray catalog) (Not yet in Simbad)
Write:	<<1EG HHMM+DDd>>
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Ref:	=1994ApJS...94..551F
by	FICHTEL C.E. , BERTSCH D.L., CHIANG J., DINGUS B.L., ESPOSITO J.A., FIERRO J.M., HARTMAN R.C., HUNTER S.D., KANBACH G., KNIFFEN D.A., KWOK P.W., LIN Y.C., MATTOX J.R., MAYER-HASSELWANDER H.A., McDONALD L., MICHELSON P.F., VON MONTIGNY C., NOLAN P.L., PINKAU K., RADECKE H.-D., ROTHERMEL H., SREEKUMAR P., SOMMER M., SCHNEID E.J., THOMPSON D.J., WILLIS T.
	Astrophys. J., Suppl. Ser., 94, 551-581 (1994)
	The first energetic γ-ray experiment telescope (EGRET) source catalog.
o	<1EG HHMM+DDd>
=E=	Catalogue in electronic form as J/ApJS/94/551
Details on Acronym: 2EG
2EG	(2nd EGRET Gamma-ray catalog)
Write:	<<2EG JHHMM+DDMM>>
N:	129
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	EGRET on the Compton Gamma Ray Observatory. Suppl. catalog: see 2EGS, sometime found as 2EG
Ref:	=1995ApJS..101..259T
by	THOMPSON D.J. , BERTSCH D.L., DINGUS B.L., ESPOSITO J.A., ETIENNE A., FICHTEL C.E., FRIEDLANDER D.P., HARTMAN R.C., HUNTER S.D., KENDIG D.J., MATTOX J.R., McDONALD L.M., VON MONTIGNY C., MUKHERJEE R., RAMANAMURTHY P.V., SREEKUMAR P., FIERRO J.M., LIN Y.C., MICHELSON P.F., NOLAN P.L., SHRIVER S.K., WILLIS T.D., KANBACH G., MAYER-HASSELWANDER H.A., MERCK M., RADECKE H.-D., KNIFFEN D.A., SCHNEID E.J.
	Astrophys. J., Suppl. Ser., 101, 259-286 (1995)
	The second EGRET catalog of high-energy γ-ray sources.
o	Table 4: <2EG JHHMM+DDMM> N=129
=E=	Catalogue in electronic form as J/ApJS/101/259
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 3EG
3EG	(3rd EGRET Gamma-ray catalog)
Write:	<<3EG JHHMM+DDMM>>
N:	271
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Data from 1991 April 22 to 1995 October 3. See the revised catalogue EGR.
Ref:	=1999ApJS..123...79H
by	HARTMAN R.C. , BERTSCH D.L., BLOOM S.D., CHEN A.W., DEINES-JONES P., ESPOSITO J.A., FICHTEL C.E., FRIEDLANDER D.P., HUNTER S.D., McDONALD L.M., SREEKUMAR P., THOMPSON D.J., JONES B.B., LIN Y.C., MICHELSON P.F., NOLAN P.L., TOMPKINS W.F., KANBACH G., MAYER-HASSELWANDER H.A., MUCKE A., POHL M., REIMER O., KNIFFEN D.A., SCHNEID E.J., VON MONTIGNY C., MUKHERJEE R., DINGUS B.L.
	Astrophys. J., Suppl. Ser., 123, 79-202 (1999)
	The third EGRET catalog of high-energy γ-ray sources.
o	<3EG JHHMM+DDMM> N=271.
=E=	Catalogue in electronic form as J/ApJS/123/79
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EG97]
[EG97]	(Eckart+Genzel, 1997)= (S)
Write:	<<[EG97] SNNNN>>
N:	112+2+1+5
Object:	* in Cl* (SIMBAD class: Star)
Note:	* in the Sgr A* cluster. See also [GEO97], [GKM98], [PGM2006], [RGH2007].
in source:	NAME Gal Center
in source:	NAME Sgr A* Cluster
Ref:	=1997MNRAS.284..576E
by	ECKART A. , GENZEL R.
	Mon. Not. R. Astron. Soc., 284, 576-598 (1997)
	Stellar proper motions in the central 0.1 pc of the Galaxy.
o	Table 2: <[EG97] SNN> (Nos S1-S11)
Ref:	=1997MNRAS.291..219G
by	GENZEL R. , ECKART A., OTT T., EISENHAUER F.
	Mon. Not. R. Astron. Soc., 291, 219-234 (1997)
	On the nature of the dark mass in the centre of the Milky Way.
o	Table 1: sources S1 to S11 = [EG97] SNN
o	Fig.1: <[EG97] S12> added. Table 1: <GCIRS 29S1>, <GCIRS 29S2> new. Table 1: <[GEO97] WNN> (Nos W1-W18).
Ref:	=2000MNRAS.317..348G
by	GENZEL R. , PICHON C., ECKART A., GERHARD O.E., OTT T.
	Mon. Not. R. Astron. Soc., 317, 348-374 (2000)
	Stellar dynamics in the Galactic Centre: proper motions and anisotropy.
o	Table 1, col(19): w217 ?? ID not identified (= [GPE2000] 1.34)
o	Table 1, col(1): <[GPE2000] NN.NNA> N=299. Table 1, col(19): <GCIRS NWWN> N=6 added. Table 1, col(19): <[EG97] SNN> (Nos S18-S19) added.
Ref:	=2003Msngr.111....1O
by	OTT T. , SCHOEDEL R., GENZEL R., ECKART A., LACOMBE F., ROUAN D., HOFMANN R., LEHNERT M., ALEXANDER T., STERNBERG A., REID M., BRANDNER W., LENZEN R., HARTUNG M., GENDRON E., CLENET Y., LENA P., ROUSSET G., LAGRANGE A.-M., AGEORGES N., HUBIN N., LIDMAN C., MOORWOOD A.F.M., RENZINI A., SPYROMILIO J., TACCONI-GARMAN L.E., MENTEN K.M., MOUAWAD N.
	The Messenger, 111, 1-8 (2003)
	Inward bound: studying the Galactic Centre with NAOS/CONICA.
o	Fig.1: <[EG97] S14> added.
Ref:	=2003ApJ...594..812G
by	GENZEL R. , SCHOEDEL R., OTT T., EISENHAUER F., HOFMANN R., LEHNERT M., ECKART A., ALEXANDER T., STERNBERG A., LENZEN R., CLENET Y., LACOMBE F., ROUAN D., RENZINI A., TACCONI-GARMAN L.E.
	Astrophys. J., 594, 812-832 (2003)
	The stellar cusp around the supermassive black hole in the Galactic Center.
o	Fig.3: <[EG97] S13> added.
Ref:	=2005ApJ...628..246E
by	EISENHAUER F. , GENZEL R., ALEXANDER T., ABUTER R., PAUMARD T., OTT T., GILBERT A., GILLESSEN S., HORROBIN M., TRIPPE S., BONNET H., DUMAS C., HUBIN N., KAUFER A., KISSLER-PATIG M., MONNET G., STROBELE S., SZEIFERT T., ECKART A., SCHODEL R., ZUCKER S.
	Astrophys. J., 628, 246-259 (2005)
	SINFONI in the Galactic Center: young stars and infrared flares in the central light-month.
o	Fig.1: <[EG97] SNN> (No. S17) added.
Ref:	=2008A&A...492..419T
by	TRIPPE S. , GILLESSEN S., GERHARD O.E., BARTKO H., FRITZ T.K., MANESS H.L., EISENHAUER F., MARTINS F., OTT T., DODDS-EDEN K., GENZEL R.
	Astron. Astrophys., 492, 419-439 (2008)
	Kinematics of the old stellar population at the Galactic centre.
o	Figure 1 Star SiO15 not identified.
o	Table 1: <[EG97] SNNN> (No. S111) added.
Ref:	=2009ApJ...692.1075G
by	GILLESSEN S. , EISENHAUER F., TRIPPE S., ALEXANDER T., GENZEL R., MARTINS F., OTT T.
	Astrophys. J., 692, 1075-1109 (2009)
	Monitoring stellar orbits around the massive black hole in the Galactic Center.
o	Fig. 1: <[EG97] SNNN> (Nos S1-S112).
o	Fig.1: Objects S1 to S112 ([EG97] SNNN) are not all in Simbad because of a lack of coordinates.
Ref:	=2017ApJ...837...30G
by	GILLESSEN S. , PLEWA P.M., EISENHAUER F., SARI R., WAISBERG I., HABIBI M., PFUHL O., GEORGE E., DEXTER J., VON FELLENBERG S., OTT T., GENZEL R.
	Astrophys. J., 837, 30-30 (2017)
	An update on monitoring stellar orbits in the Galactic Center.
o	Objects R34 and R44 are not in SIMBAD.
o	Table 2: <[EG97] SNNN> (Nos S145-146 and S175) added.
Ref:	=2020ApJ...899...50P
by	PEISSKER F. , ECKART A., ZAJACEK M., ALI B., PARSA M.
	Astrophys. J., 899, 50-50 (2020)
	S62 and S4711: indications of a population of faint fast-moving stars inside the S2 orbit - S4711 on a 7.6 yr orbit around Sgr A.*
o	<[EG97] SNNNN> (Nos S4711-S4715).
=E=	Catalogue in electronic form as <J/ApJ/837/30/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EGB
EGB	(Ellis+Grayson+Bond)= (EG B)
Write:	<<EGB NN>> <<EGB HHMM+DD>>
N:	7+3
Object:	PN or central * of PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Table 1: Definite and possible PN, N=7, not numbered with format 'N' by the authors, only format 'HHMM+DD'. Table II: additional low-surface-brightness obj,. N=3, not numbered with format 'NN' by the authors, only format 'HHMM+DD'. The objects are found in the literature renumbered from (Nos 1-10)
Ref:	=1984PASP...96..283E
by	ELLIS G.L. , GRAYSON E.T., BOND H.E.
	Publ. Astron. Soc. Pac., 96, 283-286 (1984)
	A search for faint planetary nebulae on Palomar Sky Survey prints.
o	<EGB NN> or <EGB HHMM+DD> N=10
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [EGB2019]
[EGB2019]	(Earnshaw+Grefenstette+Brightman+, 2019) (Not yet in Simbad)
Write:	<<[EGB2019] NGC 6946 ULX4>> <<[EGB2019] N>> <<[EGB2019] NGC 6946 ULX-4>> (not recognised by Simbad, but found in literature)
N:	1+6
Object:	(X) + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=1 ultraluminous X-ray sources (ULX) in XMM-Newton and NuSTAR observations of NGC 6946, and N=6 potential optical/IR counterparts from archival HST WFPC2 and WFC3/IR observations. See also [LB2005] for the first three ULXs in NGC 6946.
in source:	NGC 6946
Ref:	=2019ApJ...881...38E
by	EARNSHAW H.P. , GREFENSTETTE B.W., BRIGHTMAN M., WALTON D.J., BARRET D., FURST F., HARRISON F.A., HEIDA M., PIKE S.N., STERN D., WEBB N.A.
	Astrophys. J., 881, 38-38 (2019)
	A broadband look at the old and new ULXs of NGC 6946.
o	Fig. 1, Table 1: <[EGB2019] NGC 6946 ULX4> N=1. Fig. 11, Table 6: <[EGB2019] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EGC84]
[EGC84]	(Ellis+Gray+Carter+, 1984)
Write:	<<[EGC84] NNA>>
N:	30
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	G in the cluster containing IC 2082. Finding chart in Plate 1
in source:	IC 2082
Ref:	=1984MNRAS.206..285E
by	ELLIS R.S. , GRAY P.M., CARTER D., GODWIN J.
	Mon. Not. R. Astron. Soc., 206, 285-292 (1984)
	Multi object spectroscopy using fibre optics at the Anglo-Australian telescope - an application to the IC 2082 galaxy cluster.
o	Table 2: <[EGC84] NNA> (Nos 1A, 1B) and N=28 among (Nos 2-63)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EGE2007]
[EGE2007]	(Enoch+Glenn Evans+, 2007)= (Bolo)
Write:	<<[EGE2007] Bolo NN>>
N:	35
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Caltech Submillimeter Observatory Bolocam 1.1mm continuum survey of the Serpens cloud.
in source:	NAME Serpens Cloud
Ref:	=2007ApJ...666..982E
by	ENOCH M.L. , GLENN J., EVANS II N.J., SARGENT A.I., YOUNG K.E., HUARD T.L.
	Astrophys. J., 666, 982-1001 (2007)
	Comparing star formation on large scales in the c2d Legacy clouds: Bolocam 1.1 mm dust continuum surveys of Serpens, Perseus, and Ophiuchus.
o	Pointing source G34.3 not identified
o	Table 1: <[EGE2007] Bolo NN> (Nos 1-35).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EGG
EGG	(Evaporating Gazeous Globules)
Write:	<<EGG M16-ENN>>
N:	73
Object:	Globules (SIMBAD class: PartofCloud = Part of Cloud)
Note:	HST WFPC2 observations. Map, Plate 139
Note:	See also [PAB98], [STN2002], [FHS2002].
in source:	M 16 = Eagle Nebula = NGC 6611
Ref:	=1996AJ....111.2349H
by	HESTER J.J. , SCOWEN P.A., SANKRIT R., LAUER T.R., AJHAR E.A., BAUM W.A., CODE A., CURRIE D.G., DANIELSON G.E., EWALD S.P., FABER S.M., GRILLMAIR C.J., GROTH E.J., HOLTZMAN J.A., HUNTER D.A., KRISTIAN J., LIGHT R.M., LYNDS C.R., MONET D.G., O'NEIL E.J.Jr, SHAYA E.J., SEIDELMANN P.K., WESTPHAL J.A.
	Astron. J., 111, 2349-2360 (1996)
	Hubble Space Telescope WFPC2 imaging of M16 : photoevaporation and emerging young stellar objects.
o	Figs 1-8: <NAME M 16 PILLAR I>, <NAME M 16 PILLAR II>, <NAME M 16 PILLAR III>. Fig.8: <EGG M16-ENN> (Nos 1-73).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Eggen
Eggen	(Eggen)
*****	Avoid the usage of Eggen, prefer EGM
Origin	of the Acronym: L (1978AJ.....83.1090P)
Details on Acronym: Eggen-Greenstein
Eggen-Greenstein	(Eggen+Greenstein)
*****	Avoid the usage of Eggen-Greenstein, prefer EGGR
Details on Acronym: EGGR
EGGR	(Eggen+Greenstein)= (EG) = (Eggen-Greenstein) = (Gr)
Write:	<<EGGR NNN>>
N:	748+10
Object:	WD (SIMBAD class: WhiteDwarf = White Dwarf)
Note:	(Nos 1-266): also found named 'EG'. (Nos 267-558): also found named 'GR'. No. 21 in the catalogue corresponds to 2 objects.
Ref:	=1965ApJ...141...83E
by	EGGEN O.J. , GREENSTEIN J.L.
	Astrophys. J., 141, 83-108 (1965)
	Spectra, colors, luminosities and motions of the white dwarfs.
o	Table 1: <EGGR NNN> (Nos 1-165)
Ref:	=1965ApJ...142..925E
by	EGGEN O.J. , GREENSTEIN J.L.
	Astrophys. J., 142, 925-933 (1965)
	Observations of proper-motion stars. II.
o	Table 2: <EGGR NNN> (Nos 166-178)
Ref:	=1967ApJ...150..927E
by	EGGEN O.J. , GREENSTEIN J.L.
	Astrophys. J., 150, 927-942 (1967)
	Observations of proper-motion stars. III.
o	Table 1: <EGGR NNN> (Nos 179-202)
Ref:	=1969ApJ...158..281G
by	GREENSTEIN J.L.
	Astrophys. J., 158, 281-293 (1969)
	The Lowell suspect white dwarfs.
o	Tables 1, 2, 6: <EGGR NNN> (Nos 203-266)
Ref:	=1970ApJ...162L..55G
by	GREENSTEIN J.L.
	Astrophys. J., 162, 55-59 (1970)
	Some new white dwarfs with peculiar spectra.
o	Table 1: <EGGR NNN> (Nos 267-284)
Ref:	=1974ApJ...189L.131G
by	GREENSTEIN J.L.
	Astrophys. J., 189, 131-133 (1974)
	A new list of 52 ° stars. VII.
o	Tables 1-2: <EGGR NNN> (Nos 285-336)
Ref:	=1975ApJ...196L.117G
by	GREENSTEIN J.L.
	Astrophys. J., 196, 117-120 (1975)
	A further list of ° stars.
o	Table 1: <EGGR NNN> (Nos 337-380)
Ref:	=1976ApJ...207L.119G
by	GREENSTEIN J.L.
	Astrophys. J., 207, 119-123 (1976)
	Some further ° stars.
o	Table 1: <EGGR NNN> (Nos 381-405)
Ref:	=1977ApJ...218L..21G
by	GREENSTEIN J.L. , OKE J.B., RICHSTONE D., VAN ALTENA W.F., STEPPE H.
	Astrophys. J., 218, 21-25 (1977)
	Further ° stars.
o	Table 1: <EGGR NNN> (Nos 406-456)
Ref:	=1979ApJ...227..244G
by	GREENSTEIN J.L.
	Astrophys. J., 227, 244-251 (1979)
	A further list and some properties of red °.
o	Table 1: <EGGR NNN> (Nos 457-507)
Ref:	=1980ApJ...242..738G
by	GREENSTEIN J.L.
	Astrophys. J., 242, 738-748 (1980)
	Degenerate stars. Recognition of hot non °.
o	Table 1: <EGGR NNN> (Nos 508-558)
Ref:	=1984ApJ...276..602G
by	GREENSTEIN J.L.
	Astrophys. J., 276, 602-620 (1984)
	Spectrophotometry of the white dwarfs.
o	<EGGR NNN> (Nos 900-909)
Details on Acronym: [EGH2001]
[EGH2001]	(Eikenberry+Garske+Hu+, 2001)= ([EGH2001a])
Write:	<<[EGH2001] JHHMMSS.ss+DDMMSS.s>>
N:	3
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	N=3 possible (IR) counterparts of NAME SGR 1806-20. See also [FMC99], [EGH2001b].
Ref:	=2001IAUC.7682....2E
by	EIKENBERRY S.S. , GARSKE M., HU D., JACKSON M.A., PATEL S.G., BARRY D.J., COLONNO M., HOUCK J.R.
	IAU Circ., 7682, 2-None (2001)
	SGR 1806-20.
o	<[EGH2001] JHHMMSS.ss+DDMMSS.s> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EGH2001a]
[EGH2001a]	(Eikenberry+Garske+Hu+, 2001)
*****	Avoid the usage of [EGH2001a], prefer [EGH2001]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EGH2001b]
[EGH2001b]	(Eikenberry+Garske+Hu+, 2001)
Write:	<<[EGH2001b] N>> <<[EGH2001b] AN>>
N:	8+5+14
Object:	* (SIMBAD class: Star)
Note:	Format 'N': USNO-A2.0 calibration stars. Format 'A', 'AN': stars in the cluster [FMC99] B near SGR 1806-20. See also FMC99], [EGH2001].
Ref:	=2001ApJ...563L.133E
by	EIKENBERRY S.S. , GARSKE M.A., HU D., JACKSON M.A., PATEL S.G., BARRY D.J., COLONNO M.R., HOUCK J.R.
	Astrophys. J., 563, 133-137 (2001)
	Possible infrared counterparts to the soft γ-ray repeater Sgr 1806-20.
o	Fig.2: <[EGH2001b] N> (Nos 1-8). Fig.2, Table 1: <[EGH2001b] A> (Nos A-E).
Ref:	=2005ApJ...623L.125K
by	KOSUGI G. , OGASAWARA R., TERADA H.
	Astrophys. J., 623, 125-128 (2005)
	A variable infrared counterpart to the soft γ-ray repeater Sgr 1806-20.
o	Fig.2, Table 1: <[EGH2001b] AN> (Nos A1-A4, B1-B3, F1-F7) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EGIPS
EGIPS	(Edge-on Galaxies In the Pan-STARRS survey) (Not yet in Simbad)
Write:	<<EGIPS JHHMMSS.s+DDMMSS>>
N:	18314
Object:	G (SIMBAD class: Galaxy)
Note:	N=18314 edge-on galaxy candidates in the Pan-STARRS DR2 survey. More information is available on the project website: https://www.sao.ru/edgeon/catalogs.php?cat=PS1candidate See also EON.
Ref:	=2022MNRAS.511.3063M
by	MAKAROV D. , SAVCHENKO S., MOSENKOV A., BIZYAEV D., RESHETNIKOV V., ANTIPOVA A., TIKHONENKO I., USACHEV P., BORISOV S., MAKAROVA L., KAUTSCH S., MARCHUK A., RUBTSOV E.
	Mon. Not. R. Astron. Soc., 511, 3063-3075 (2022)
	The edge-on Galaxies in the Pan-STARRS survey (EGIPS).
o	<EGIPS JHHMMSS.s+DDMMSS> N=16551.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EGK2020]
[EGK2020]	(Escala+Gilbert+Kirby+, 2020)
Write:	<<[EGK2020] NNNNNNN>>
N:	129
Object:	RGB* (SIMBAD class: RGB* = Red Giant Branch star)
Stat:	is completely incorporated in Simbad
Note:	Keck DEIMOS observations of N=129 red giant branch (RGB) stars in the outer disk, giant stellar stream, and inner halo of M31. See also [EKG2019], [GKE2019], and [EKG2020].
in source:	NGC 224 = M 31
in source:	NAME Andromeda Stream
Ref:	=2020ApJ...889..177E
by	ESCALA I. , GILBERT K.M., KIRBY E.N., WOJNO J., CUNNINGHAM E.C., GUHATHAKURTA P.
	Astrophys. J., 889, 177-177 (2020)
	Elemental abundances in M31: a comparative analysis of α and iron element abundances in the the outer disk, Giant Stellar Stream, and inner halo of M31.
o	Table 6: <[EGK2020] NNNNNNN> N=129 among (Nos 2493-3000724).
=E=	Catalogue in electronic form as <J/ApJ/889/177/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EGM
EGM	(Eggen, proper Motion)= (Eggen)
Write:	<<EGM NNN>> <<EGM NNNb>> <<EGM NNNA>> <<EGM NNNAB>> <<EGM NNNbA>>
N:	822+13+53
Object:	PM* (SIMBAD class: HighPM* = High Proper Motion Star)
Note:	Table 1: (Nos 1-823), No. 35 missing. Table 2: supplementary list, N=13 stars format 'NNNb'. Tables 3, 4: N=52 stars are pairs, format 'NNNA', 'NNNAB', NNNbA'
Ref:	=1976ApJS...30..351E
by	EGGEN O.J.
	Astrophys. J., Suppl. Ser., 30, 351-396 (1976)
	Stellar population samples at the galactic poles. III. UBVRI observations of proper motion stars near the south pole and the luminosity laws for the halo and old disk populations.
o	Table 1: <EGM NNN> (Nos 1-823), No. 35 missing. Table 2: <EGM NNNb> N=13. Tables 3, 4: <EGM NNNA>, <EGM NNNAB>, <EGM NNNbA> N=53
Details on Acronym: [EGM92]
[EGM92]	(Eiroa+Gomez de Castro+Miranda, 1992)
Write:	<<[EGM92] Star NN>> <<[EGM92] GGD NNA>> <<[EGM92] GGD 32-NA>>
N:	13+11+11
Object:	* + Component (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Calar Alto 3.5m telescope observations. N=13 stars in NGC 7129 field, format 'Star NN', but also designated as 'Cl* NGC 7129 EGM NN'. Components 'GGD NNA' for GGD 32, GGD 33, GGD 34 and GGD 35. Clumps 'NA' in GGD 32.
in source:	NGC 7129
Ref:	=1992A&AS...92..721E
by	EIROA C. , GOMEZ DE CASTRO A.I., MIRANDA L.F.
	Astron. Astrophys., Suppl. Ser., 92, 721-728 (1992)
	Herbig-Haro objects in the star formation region NGC 7129.
o	GGD 33 has 2 components already noted in 1978ApJ.224L.137G, and then found in literature as GGD 33a and GGD 33b, [EGM92] GGD 33A and [EGM92] GGD 33B in SIMBAD.
o	Table 2: <Cl* NGC 7129 EGM NN> (Nos 1-13) = <[EGM92] Star NN> (Nos 1-13), <[EGM92] GGD NNA> N=3+2+3+3, <[EGM92] GGD 32-NA> N=11.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EGNoG
EGNoG	(Evolution of molecular Gas in Normal Galaxies)
Write:	<<EGNoG ANN>>
N:	31
Object:	G (SIMBAD class: Galaxy)
Note:	CARMA CO(1-0) and CO(3-2) in the 3mm and 1mm bands observations of N=31 galaxies from z=0.05 to z=0.5.
Ref:	=2013ApJ...768..132B
by	BAUERMEISTER A. , BLITZ L., BOLATTO A., BUREAU M., LEROY A., OSTRIKER E., TEUBEN P., WONG T., WRIGHT M.
	Astrophys. J., 768, 132 (2013)
	The EGNoG survey: molecular gas in intermediate-redshift star-forming galaxies.
o	Figs 3-8, Tables 2-3: <EGNoG ANN> (Nos A1-A13, B1-B10, C1-C4, D1-D4).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EGO
EGO	(Extended Green Object)
Write:	<<EGO GLLL.ll+B.bb>> <<EGO GLLL.ll+B.bb(a)>> <<EGO GLLL.ll+B.bb O-W>>
N:	304+98
Object:	Extended Green Object (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Extended 4.5mu.m sources in Spitzer GLIMPSE data.
Ref:	=2008AJ....136.2391C
by	CYGANOWSKI C.J. , WHITNEY B.A., HOLDEN E., BRADEN E., BROGAN C.L., CHURCHWELL E., INDEBETOUW R., WATSON D.F., BABLER B.L., BENJAMIN R., GOMEZ M., MEADE M.R., POVICH M.S., ROBITAILLE T.P., WATSON C.
	Astron. J., 136, 2391-2412 (2008)
	A catalog of extended green objects in the GLIMPSE survey: a new sample of massive young stellar object outflow candidates.
o	Tables 1-5: <EGO GLLL.ll+B.bb(a)>, <EGO GLLL.ll+B.bb O-W>, N=304.
Ref:	=2013ApJS..206....9C
by	CHEN X. , GAN C.-G., ELLINGSEN S.P., HE J.-H., SHEN Z.-Q., TITMARSH A.
	Astrophys. J., Suppl. Ser., 206, 9 (2013)
	Newly identified extended green objects (EGOs) from the Spitzer GLIMPSE II survey. I. Catalog.
o	Tables 1+2+4: <EGO GLLL.ll+BB.bb(a)> N=98.
=E=	Catalogue in electronic form as <J/AJ/136/2391/>
=E=	Catalogue in electronic form as <J/ApJS/206/9/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EGR
EGR	(EGRET Revised)
Write:	<<EGR JHHMM+DDMM>>
N:	174
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Revised catalogue of gamma-ray sources detected by EGRET detector on the Compton Gamma-Ray Observatory. See also EGRc. Previous catalogues: 1EG, 2EG, 3EG.
Ref:	=2008A&A...489..849C
by	CASANDJIAN J.-M. , GRENIER I.A.
	Astron. Astrophys., 489, 849-883 (2008)
	A revised catalogue of EGRET γ-ray sources.
o	Tables A1, B1, col(1): numbering NNN not used in SIMBAD.
o	Table A1: <EGR JHHMM+DDMM> N=174. Table B1: <EGRc JHHMM+DDMM> N=14.
=E=	Catalogue in electronic form as J/A+A/489/849
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EGRc
EGRc	(EGRET Revised, confused source)
Write:	<<EGRc JHHMM+DDMM>>
N:	14
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	Revised catalogue of gamma-ray sources detected by EGRET detector on the Compton Gamma-Ray Observatory, confused sources. See also the complete catalogue: EGR.
Ref:	=2008A&A...489..849C
by	CASANDJIAN J.-M. , GRENIER I.A.
	Astron. Astrophys., 489, 849-883 (2008)
	A revised catalogue of EGRET γ-ray sources.
o	Tables A1, B1, col(1): numbering NNN not used in SIMBAD.
o	Table A1: <EGR JHHMM+DDMM> N=174. Table B1: <EGRc JHHMM+DDMM> N=14.
=E=	Catalogue in electronic form as J/A+A/489/849
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EGS
EGS	(Extended Groth Strip sources) >>>>>> New acronym being registered
Object:	?
in source:	NAME Extended Groth Strip
Auth.:	NEWMAN J.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: EGS06
EGS06	(Extended Groth Strip, 2006)
Write:	<<EGS06 NN>>
N:	51
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA 6cm observations of the Extended Groth Strip (EGS).
in source:	NAME Extended Groth Strip
Ref:	=2006AJ....132.2159W
by	WILLNER S.P. , COIL A.L., GOSS W.M., ASHBY M.L.N., BARMBY P., HUANG J.-S., IVISON R., KOO D.C., EGAMI E., MIYAZAKI S.
	Astron. J., 132, 2159-2170 (2006)
	Mid-infrared identification of 6 cm radio-source counterparts in the Extended Groth Strip.
o	Table 1: <EGS06 NN> (Nos 1-51).
=E=	Catalogue in electronic form as J/AJ/132/2159
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 2EGS
2EGS	(2nd EGRET Gamma-ray catalog, Suppl.)
Write:	<<2EGS JHHMM+DDMM>>
N:	28
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	EGRET on the Compton Gamma Ray Observatory, additional 28 sources to the 2EG catalog. Sometime found named 2EG
Ref:	=1996ApJS..107..227T
by	THOMPSON D.J. , BERTSCH D.L., DINGUS B.L., ESPOSITO J.A., ETIENNE A., FICHTEL C.E., FRIEDLANDER D.P., HARTMAN R.C., HUNTER S.D., KENDIG D.J., MATTOX J.R., McDONALD L.M., MUKHERJEE R., RAMANAMURTHY P.V., SREEKUMAR P., VON MONTIGNY C., FIERRO J.M., JONES B.B., LIN Y.C., MICHELSON P.F., NOLAN P.L., TOMPKINS W., WILLIS T.D., KANBACH G., MAYER-HASSELWANDER H.A., MERCK M., POHL M., KNIFFEN D.A., SCHNEID E.J.
	Astrophys. J., Suppl. Ser., 107, 227-237 (1996)
	Supplement to the second EGRET catalog of high-energy γ-ray sources.
o	Table 2: <2EGS JHHMM+DDMM> N=28
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EGS20
EGS20	(Extended Groth Strip international survey at 20cm) (Not yet in Simbad)
Write:	<<EGS20 JHHMMSS.ss+DDMMSS.s>>
N:	about 1200
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	In preparation. VLA 1.4-GHz radio survey of the Extended Groth Strip: The 20cm is one of a number of panchromatic surveys.
Auth.:	IVISON R.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [EGS2015]
[EGS2015]	(Einasto+Gramann+Saar+, 2015)
Write:	<<[EGS2015] NN>>
N:	14
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=14 galaxy groups in the A2142 supercluster. Use of SDSS DR8 and DR10 data.
in source:	ACO 2142
Ref:	=2015A&A...580A..69E
by	EINASTO M. , GRAMANN M., SAAR E., LIIVAMAGI L.J., TEMPEL E., NEVALAINEN J., HEINAEMAEKI P., PARK C., EINASTO J.
	Astron. Astrophys., 580A, 69-69 (2015)
	Unusual A2142 supercluster with a collapsing core: distribution of light and mass.
o	Table 2: <[EGS2015] NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EGS70
EGS70	(Extended Groth Strip, at 70mu.m)
Write:	<<EGS70 NNN>>
N:	43
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Spitzer MIPS 70mu.m survey of the Extended Groth Strip. 2008MNRAS.385.1015S: N=43 selected high-redshift galaxies. 2010MNRAS.403.1474S: N=61 galaxies.
in source:	NAME Extended Groth Strip
Ref:	=2008MNRAS.385.1015S
by	SYMEONIDIS M. , WILLNER S.P., RIGOPOULOU D., HUANG J.-S., FAZIO G.G., JARVIS M.J.
	Mon. Not. R. Astron. Soc., 385, 1015-1028 (2008)
	The properties of 70 µm-selected high-redshift galaxies in the Extended Groth Strip.
o	Table 1: <EGS70 NNN> N=43 among (Nos 41-172).
Ref:	=2010MNRAS.403.1474S
by	SYMEONIDIS M. , ROSARIO D., GEORGAKAKIS A., HARKER J., LAIRD E.S., PAGE M.J., WILLMER C.N.A.
	Mon. Not. R. Astron. Soc., 403, 1474-1490 (2010)
	The central energy source of 70 µm-selected galaxies: starburst or AGN ?
o	Table 4: <EGS70 NNN> N=61 among (Nos 20-172).
=E=	Catalogue in electronic form as J/MNRAS/403/1474
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EGSD2
EGSD2	(Extended Groth Strip, DEEP2 survey)
Write:	<<EGSD2 JHHMMSS.ss+DDMMSS.s>> <<EGSD2 JHHMMSS.s+DDMMSS>>
N:	1+20
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Photometric catalog of the Extended Groth Strip from the DEEP2 Galaxy Redshift Survey. 2007ApJ...660L..23G: first ref. with an EGSD2 galaxy.
Auth.:	GERKE B.
Ref:	=2007ApJ...660L..23G
by	GERKE B.F. , NEWMAN J.A., LOTZ J., YAN R., BARMBY P., COIL A.L., CONSELICE C.J., IVISON R.J., LIN L., KOO D.C., NANDRA K., SALIM S., SMALL T., WEINER B.J., COOPER M.C., DAVIS M., FABER S.M., GUHATHAKURTA P.
	Astrophys. J., 660L, 23-26 (2007)
	The DEEP2 Galaxy Redshift Survey: AEGIS observations of a dual AGN at z = 0.7.
o	<EGSD2 JHHMMSS.ss+DDMMSS.s> N=1.
Ref:	=2009ApJ...698..956C
by	COMERFORD J.M. , GERKE B.F., NEWMAN J.A., DAVIS M., YAN R., COOPER M.C., FABER S.M., KOO D.C., COIL A.L., ROSARIO D.J., DUTTON A.A.
	Astrophys. J., 698, 956-965 (2009)
	Inspiralling supermassive black holes: a new signpost for galaxy mergers.
o	Table 1: <EGSD2 JHHMMSS.s+DDMMSS> N=20, <DEEP2 JHHMMSS.s+DDMMSS> N=12.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: EGSIRAC
EGSIRAC	(Extended Groth Strip, IRAC)
Write:	<<EGSIRAC JHHMMSS.ss+DDMMSS.s>>
N:	57434
Object:	(Mid IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Spitzer IRAC observations of the Extended Groth Strip.
in source:	NAME Extended Groth Strip
Ref:	=2008ApJS..177..431B
by	BARMBY P. , HUANG J.-S., ASHBY M.L.N., EISENHARDT P.R.M., FAZIO G.G., WILLNER S.P., WRIGHT E.L.
	Astrophys. J., Suppl. Ser., 177, 431-445 (2008)
	A catalog of mid-infrared sources in the Extended Groth Strip.
o	Table 6: <EGSIRAC JHHMMSS.ss+DDMMSS.s> N=57434.
=E=	Catalogue in electronic form as J/ApJS/177/431
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EGT95]
[EGT95]	(Ettori+Guzzo+Tarenghi, 1995)
Write:	<<[EGT95] HHMMSS.s+DDMMSS>>
N:	about 600
Object:	G (SIMBAD class: Galaxy)
Ref:	=1995MNRAS.276..689E
by	ETTORI S. , GUZZO L., TARENGHI M.
	Mon. Not. R. Astron. Soc., 276, 689-705 (1995)
	A study of the large-scale distribution of galaxies in the South Galactic Pole region - I. The data.
o	Tables 4(a) to (e): <[EGT95] HHMMSS.s-DDMMSS> N about 600
=E=	Catalogue in electronic form as J/MNRAS/276/689
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EGY91]
[EGY91]	(Ellington+Green+Yee, 1991)
Write:	<<[EGY91] PKS HHMM+DDd MaskNNN NN>> <<[EGY91] PKS HHMM+DDd NN>> <<[EGY91] PG HHMM+DD MaskNNN NN>> <<[EGY91] PG HHMM+DDd NN>> <<[EGY91] PG HHMM+DD NN>> <<[EGY91] 4C DD.NN NN>> <<[EGY91] 3C NNN MaskNNN NN>> <<[EGY91] 3C NNN NN>>
N:	261
Object:	G + * + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 2: N=261 spectra in 17 fields of QSO, among which N=127 galaxies, N=28 stars, others are unidentified. Some fields are observed with 2 differents masks, each mask with a format 'NNN', and in this case objects have a format: 'QSO HHMM+DDd MaskNNN NN'. See also Paper I: [EYG89]
Ref:	=1991ApJ...378..476E
by	ELLINGSON E. , GREEN R.F., YEE H.K.C.
	Astrophys. J., 378, 476-486 (1991)
	Clusters of galaxies associated with quasars. II. Galaxy cluster dynamics.
o	Table 2: <[EGY91] PKS HHMM+DDd MaskNNN NN>, <[EGY91] PKS HHMM+DDd NN>, <[EGY91] PG HHMM+DD MaskNNN NN>, <[EGY91] PG HHMM+DDd NN>, <[EGY91] PG HHMM+DD NN>, <[EGY91] 4C DD.NN NN, <[EGY91] 3C NNN MaskNNN NN>, <[EGY91] 3C NNN NN> N=261
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EH2001]
[EH2001]	(Everett+Howell, 2001) (Not yet in Simbad)
Write:	<<[EH2001] a>>
N:	4
Object:	* (SIMBAD class: Star)
Ref:	=2001PASP..113.1428E
by	EVERETT M.E. , HOWELL S.B.
	Publ. Astron. Soc. Pac., 113, 1428-1435 (2001)
	A technique for ultrahigh-precision CCD photometry.
o	Table 1: <[EH2001] a> (Nos a-d).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EHB2020]
[EHB2020]	(Earnshaw+Heida+Brightman+, 2020)
Write:	<<[EHB2020] NGC 925 ULX-3>>
N:	1
Object:	ULX (SIMBAD class: ULX = Ultra-luminous X-ray Source)
Note:	Chandra ACIS observations of N=1 ULX in NCG 925. Use of archival Swift, XMM-Newton, and NuSTAR data.
in source:	NGC 925
Ref:	=2020ApJ...891..153E
by	EARNSHAW H.P. , HEIDA M., BRIGHTMAN M., FURST F., HARRISON F.A., JAODAND A., MIDDLETON M.J., ROBERTS T.P., SATHYAPRAKASH R., STERN D., WALTON D.J.
	Astrophys. J., 891, 153-153 (2020)
	The (re)appearance of NGC 925 ULX-3, a new transient ULX.
o	<[EHB2020] NGC 925 ULX-3> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EHC2008]
[EHC2008]	(Elsner+Heinke+Cohn+, 2008)
Write:	<<[EHC2008] sNN>> <<[EHC2008] ssNN>> <<[EHC2008] isNN>>
N:	63+39+14
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of M 71.
in source:	M 71 = NGC 6836
Ref:	=2008ApJ...687.1019E
by	ELSNER R.F. , HEINKE C.O., COHN H.N., LUGGER P.M., MAXWELL J.E., STAIRS I.H., RANSOM S.M., HESSELS J.W.T., BECKER W., HUANG R.H.H., EDMONDS P.D., GRINDLAY J.E., BOGDANOV S., GHOSH K., WEISSKOPF M.C.
	Astrophys. J., 687, 1019-1034 (2008)
	Chandra X-ray observatory observations of the globular cluster M71.
o	Table 1: <[EHC2008] sNN> (Nos s1-s63). Table 2: <[EHC2008] ssNN> (Nos ss1-ss39), <[EHC2008] isNN> (Nos is1-is14).
=E=	Catalogue in electronic form as <J/ApJ/687/1019/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EHE2003]
[EHE2003]	(Einasto+Husti+Einasto+, 2003)
Write:	<<[EHE2003] WNNA>>
N:	16+24+3
Object:	Cl of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	SDSS Early Data Release survey is used to extract clusters and groups of galaxies. See also [EEH2003] for superclusters.
Ref:	=2003A&A...405..425E
by	EINASTO J. , HUETSI G., EINASTO M., SAAR E., TUCKER D.L., MUELLER V., HEINAEMAEKI P., ALLAM S.S.
	Astron. Astrophys., 405, 425-443 (2003)
	Clusters and superclusters in the Sloan Digital Sky Survey.
o	Table 3: <[EHE2003] WNNA> (Nos S01-S16, N01-N24, N10A-N10C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EHG2002]
[EHG2002]	(Edmonds+Heinke+Grindlay+, 2002) (Not yet in Simbad)
Write:	<<[EHG2002] CN>> <<[EHG2002] NN>>
N:	3+3
Object:	* (SIMBAD class: Star)
Note:	Chandra and HST images of 47 Tuc. N=3 stars in the error box of [HJV94] 5. N=3 stars in the error box of [HJV94] 7. See [HJV94].
in source:	NGC 104 = 47 Tuc
Ref:	=2002ApJ...564L..17E
by	EDMONDS P.D. , HEINKE C.O., GRINDLAY J.E., GILLILAND R.L.
	Astrophys. J., 564, 17-20 (2002)
	Hubble space telescope detection of a quiescent low-mass X-ray binary companion in 47 Tucanae.
o	X5, X7 in 47 Tuc are [HJV94] 5, ...7, qLMXB in NGC 6397 is CGKB B
o	Text: <[EHG2002] AN> (Nos C1-C3, N1-N3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EHM2007]
[EHM2007]	(Ellison+Hennawi+Martin+, 2007) (Not yet in Simbad)
Write:	<<[EHM2007] QSO J1116+4118A abs N.NN>> <<[EHM2007] QSO J1116+4118A abs N.NNNN>>
N:	3+3
Object:	DLA
Ref:	=2007MNRAS.378..801E
by	ELLISON S.L. , HENNAWI J.F., MARTIN C.L., SOMMER-LARSEN J.
	Mon. Not. R. Astron. Soc., 378, 801-818 (2007)
	Coincident, 100 kpc scale damped Lyα absorption towards a binary QSO: how large are galaxies at z ~ 3?
o	<[EHM2007] QSO J1116+4118A abs N.NN>, <[EHM2007] QSO J1116+4118A abs N.NNNN> N=1+2, <[EHM2007] QSO J1116+4118B abs N.NN>, <[EHM2007] QSO J1116+4118B abs N.NNNN> N=1+2,
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EHR
EHR	(Extraplanar HII Region)
Write:	<<EHR N>>
N:	2
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	UT1 FORS1 VLT observations. N=2 extraplanar HII regions in the field of NGC 55.
Ref:	=2003A&A...412...69T
by	TUELLMANN R. , ROSA M.R., ELWERT T., BOMANS D.J., FERGUSON A.M.N., DETTMAR R.-J.
	Astron. Astrophys., 412, 69-80 (2003)
	Star formation in gaseous galaxy halos. VLT-spectroscopy of extraplanar HII-regions in NGC 55.
o	Figs 1, 2: <EHR N> (Nos 1-2).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EHV2002]
[EHV2002]	(Everett+Howell+Van Belle+, 2002)
Write:	<<[EHV2002] F-N-NNNN>>
N:	222
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Statistical study, N=222 variable stars. In the format 'F' stands for field number (1 or 2), 'N' stands for a CCD number (1 to 8), and 'NNNN' stands for a numbering of each star detected in a CCD.
Ref:	=2002PASP..114..656E
by	EVERETT M.E. , HOWELL S.B., VAN BELLE G.T., CIARDI D.R.
	Publ. Astron. Soc. Pac., 114, 656-670 (2002)
	Stellar variability in a survey of field stars.
o	Table 2: <[EHV2002] F-N-NNN> N=222.
=E=	Catalogue in electronic form as J/PASP/114/656
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EHVHCOP
EHVHCOP	(Extr. High Velocity, HCO+)
Write:	<<EHVHCOP N>>
N:	3
Object:	Clump (SIMBAD class: HVCld = High-velocity Cloud)
Stat:	is completely incorporated in Simbad
in source:	NAME HH 7-11
Ref:	=1996ApJ...462..355M
by	MEHRINGER D.M.
	Astrophys. J., 462, 355-363 (1996)
	The location of extremely high velocity HCO^+ in the HH 7-11 outflow.
o	SVS 13 = [SVS76] NGC 1333 13. Table 2: peaks in clumps are not in Simbad
o	Table 1: <EHVHCOP N> (Nos 1-3)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: eHWC
eHWC	(HAWC Observatory high-energy catalog) >>>>>> New acronym being registered
Object:	(Gamma)
Ref:	=2019ICRC...36..734M
Auth.:	Kelly Malone
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: eHWC
eHWC	(energy-HAWC)
Write:	<<eHWC JHHMM+DDd>>
N:	9
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	The first catalog of TeV gamma-ray sources emitting above 56TeV observed by the High Altitude Water Cherenkov Observatory (http://www.hawc-observatory.org).
Ref:	=2020PhRvL.124b1102A
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EI
EI	(Einstein IPC)
*****	Avoid the usage of EI, prefer WW
Origin	of the Acronym: L (2000A&A...359..573H)
Details on Acronym: [EI87]
[EI87]	(Efremov+Ivanov, 1987)
Write:	<<[EI87] N>>
N:	9
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Finding chart
in source:	M 31 = NGC 224
Ref:	=1987Ap&SS.129...39E
by	EFREMOV Y.N. , IVANOV G.R.
	Astrophys. Space Sci., 129, 39-43 (1987)
	The luminosity of red supergiants in the Andromeda galaxy.
o	Table I: <[EI87] N> (Nos 1-9)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EI97]
[EI97]	(English+Irwin, 1997) (Not yet in Simbad)
Write:	<<[EI97] NN>>
N:	20
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Map in Fig.5
in source:	NGC 3432
Ref:	=1997AJ....113.2006E
by	ENGLISH J. , IRWIN J.A.
	Astron. J., 113, 2006-2024 (1997)
	The ionized gas and radio halo of NGC 3432 (ARP 206).
o	Table 4: HII regions not in SIMBAD
o	Table 4: <[EI97] NN> (Nos 1-20)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EIC
EIC	(Equatorial Infrared Catalog)
Write:	<<EIC NNNNN>>
N:	7220
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Sources detected at 2.7 mu.m. \|b\| < 10deg. 1st parution: Sweeney+ 1978, Aerospace Corporation TR-0078(3409-20)-1, (Nos 1-896). Complete catalogue, N=11214 is an electronic catalogue: Equatorial Infrared Catalog (Sweeney+ 1990), result of additional processing of USAF satellite data.
Auth.:	SWEENEY L.H.+
=E=	Catalogue in electronic form as II/161
Details on Acronym: [EIP2004]
[EIP2004]	(Ellison+Ibata+Pettini+, 2004)
Write:	<<[EIP2004] QSO J0831+5245 abs N.NNN>> <<[EIP2004] NN>>
N:	29
Object:	Absorber
Note:	HST STIS observations. List of intervening absorbers in the spectra of QSO J0831+5245 = NAME APM 08279+5255. See also [IIL98], [PAS2000].
Ref:	=2004A&A...414...79E
by	ELLISON S.L. , IBATA R., PETTINI M., LEWIS G.F., ARACIL B., PETITJEAN P., SRIANAND R.
	Astron. Astrophys., 414, 79-93 (2004)
	The sizes and kinematic structure of absorption systems towards the lensed quasar APM08279+5255.
o	Table 2: <[EIP2004] QSO J0831+5245 abs N.NNN> N=29, <[EIP2004] NN> (Nos 1-40).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EIRS
EIRS	(ELAIS-IRS sample)
Write:	<<EIRS NN>>
N:	70
Object:	IR luminous G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRS observations of N=70 infrared-luminous galaxies from the ELAIS Survey.
Ref:	=2009MNRAS.395.1695H
by	HERNAN-CABALLERO A. , PEREZ-FOURNON I., HATZIMINAOGLOU E., AFONSO-LUIS A., ROWAN-ROBINSON M., RIGOPOULOU D., FARRAH D., LONSDALE C.J., BABBEDGE T., CLEMENTS D., SERJEANT S., POZZI F., VACCARI M., MONTENEGRO-MONTES F.M., VALTCHANOV I., GONZALEZ-SOLARES E., OLIVER S., SHUPE D., GRUPPIONI C., VILA-VILARO B., LARI C., FRANCA F.L.
	Mon. Not. R. Astron. Soc., 395, 1695-1722 (2009)
	Mid-infrared spectroscopy of infrared-luminous galaxies at z ~ 0.5-3.
o	Tables 1-8, 12: <EIRS NN> (Nos 1-70).
=E=	Catalogue in electronic form as J/MNRAS/395/1695
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EIS
EIS	(ESO Imaging Survey)
*****	Avoid the usage of EIS, prefer [CAA2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EIS
EIS	(ESO Imaging Survey)
*****	Avoid the usage of EIS, prefer [DSO99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EIS
EIS	(ESO Imaging Survey)
Write:	<<EIS JHHMMSS.ss+DDMMSS.s>>
N:	42087+37093+74827+45912+65148+43253
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	ESO-MPG 2.2m WFI observations. The EIS is described in 1997Msngr..87...23R and 1999A&AS..137...51N. There are 7 catalogs for the 7 passbands.
in source:	NAME CDFS
Ref:	=2001A&A...379..740A
by	ARNOUTS S. , VANDAME B., BENOIST C., GROENEWEGEN M.A.T., DA COSTA L., SCHIRMER M., MIGNANI R.P., SLIJKHUIS R., HATZIMINAOGLOU E., HOOK R., MADEJSKY R., RITE C., WICENEC A.
	Astron. Astrophys., 379, 740-754 (2001)
	ESO imaging survey. Deep public survey: Multi-color optical data for the Chandra Deep Field South.
o	Catalogue: <EIS JHHMMSS.ss+DDMMSS.s> N=42087+37093+74827+45912+65148+43253.
=E=	Catalogue in electronic form as J/A+A/379/740
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EIS
EIS	(ESO Imaging Survey)
Note:	EIS catalogue in Chandra Deep Field South.
*****	Avoid the usage of EIS, prefer [GGH2002]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EIS
EIS	(ESO Imaging Survey)
*****	Avoid the usage of EIS, prefer [HGD2002]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EIS
EIS	(ESO Imaging Survey)
*****	Avoid the usage of EIS, prefer [KW2001b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EIS
EIS	(ESO Imaging Survey)
*****	Avoid the usage of EIS, prefer [OSD99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EIS
EIS	(ESO Imaging Survey)
*****	Avoid the usage of EIS, prefer [RBB2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EIS
EIS	(ESO Imaging Survey)
*****	Avoid the usage of EIS, prefer [RPF2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EIS
EIS	(ESO Imaging Survey)
*****	Avoid the usage of EIS, prefer [SOD99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EIS
EIS	(ESO Imaging Survey)
*****	Avoid the usage of EIS, prefer [ZHM99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EIS-DEEP
EIS-DEEP	(ESO Imaging Survey, Deep)
Write:	<<EIS-DEEP CDFS-N A N NNNN>> <<EIS-DEEP CDFS-N Aa N NNNN>> <<EIS-DEEP HDFS-N A N NNNN>> <<EIS-DEEP HDFS-N Aa N NNNN>>
N:	7735
Object:	(IR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Stat:	is completely incorporated in Simbad
Note:	ESO NTT NIR observations of the HDFS and CDFS.
in source:	NAME HDFS
in source:	NAME CDFS
Ref:	=2006A&A...452..119O
by	OLSEN L.F. , MIRALLES J.-M., DA COSTA L., BENOIST C., VANDAME B., RENGELINK R., RITE C., SCODEGGIO M., SLIJKHUIS R., WICENEC A., ZAGGIA S.
	Astron. Astrophys., 452, 119-129 (2006)
	ESO imaging survey: infrared observations of CDF-S and HDF-S.
o	Catalog: <EIS-DEEP CDFS-N A N NNNN>,<EIS-DEEP CDFS-N Aa N NNNN>, <EIS-DEEP HDFS-N A N NNNN>, <EIS-DEEP HDFS-N Aa N NNNN>, N=7735.
=E=	Catalogue in electronic form as J/A+A/452/119
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EIS-DEEP
EIS-DEEP	(ESO Imaging Survey, Deep)
*****	Avoid the usage of EIS-DEEP, prefer EIS-DPS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EIS-DPS
EIS-DPS	(ESO Imaging Survey, Deep Public Survey)
Write:	<<EIS-DPS Na NNNNN>>
N:	270434+243525+433540
Object:	(IR) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	ESO Deep Public Survey, part of the ESO Imaging Survey (EIS).
Ref:	=2007A&A...462..553M
by	MIGNANO A. , MIRALLES J.-M., DA COSTA L., OLSEN L.F., PRANDONI I., ARNOUTS S., BENOIST C., MADEJSKY R., SLIJKHUIS R., ZAGGIA S.
	Astron. Astrophys., 462, 553-563 (2007)
	ESO imaging survey: optical deep public survey.
o	(Erratum) erratum vol. 466, p. 541 (2007)
o	Catalog: <EIS-DPS Na NNNNN> N=270434+243525+433540.
=E=	Catalogue in electronic form as J/A+A/462/553
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EISD
EISD	(ESO Imaging Survey, Patch D)
Write:	<<EISD NNN>>
N:	199
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	New sample of radio-sources defined by combining the NVSS and the EIS survey. See also CENSORS.
Ref:	=2003MNRAS.346..627B
by	BEST P.N. , ARTS J.N., ROETTGERING H.J.A., RENGELINK R., BROOKES M.H., WALL J.
	Mon. Not. R. Astron. Soc., 346, 627-683 (2003)
	CENSORS: A Combined EIS-NVSS Survey Of Radio Sources - I. Sample definition, radio data and optical identifications.
o	Table A1: <EISD NNN> (Nos 1-199). Table C1: <CENSORS NNN> (Nos 1-150), <CENSORS XN> (Nos X1-X3), <CENSORS D1> N=1.
=E=	Catalogue in electronic form as J/MNRAS/346/627
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EJF2001]
[EJF2001]	(Ebeling+Jones+Fairley+, 2001)
Write:	<<[EJF2001] A>>
N:	6
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	ROSAT WARPS survey. Map in Fig.1.
in source:	WARPS J1226.0+3332
Ref:	=2001ApJ...548L..23E
by	EBELING H. , JONES L.R., FAIRLEY B.W., PERLMAN E., SCHARF C., HORNER D.
	Astrophys. J., 548, 23-27 (2001)
	Discovery of a very X-ray luminous galaxy cluster at z=0.89 in the wide angle ROSAT pointed survey.
o	Table 1: <[EJF2001] A> (Nos A-F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EJP2000]
[EJP2000]	(Ebeling+Jones+Perlman+, 2000)
Write:	<<[EJP2000] A>>
N:	6
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Wide angle ROSAT pointed survey (WARPS). N=6 galaxies, members of the ClG RX J0152.7-1357. Identif. chart in Fig.2.
in source:	RX J0152.7-1357 = ClG J0152-1357
Ref:	=2000ApJ...534..133E
by	EBELING H. , JONES L.R., PERLMAN E., SCHARF C., HORNER D., WEGNER G., MALKAN M., FAIRLEY B.W., MULLIS C.R.
	Astrophys. J., 534, 133-145 (2000)
	The WARPS survey. III. The discovery of an X-ray luminous galaxy cluster at z=0.833 and the impact of X-ray substructure on cluster abundance measurements.
o	Table 1: <[EJP2000] A> (Nos A-F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EK2000]
[EK2000]	(Elias+Koch, 2000) (Not yet in Simbad)
Write:	<<[EK2000] NN>>
N:	18
Object:	* (SIMBAD class: Star)
Note:	N=18 comparison stars. Image in Fig.1.
Ref:	=2000AJ....120.1548E
by	ELIAS II N.M. , KOCH R.H.
	Astron. J., 120, 1548-1553 (2000)
	Photospheric spots and a chromospheric plage on V523 Cassiopeiae.
o	Fig.1, Table 2: <[EK2000] NN> (Nos 1-18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EK2019]
[EK2019]	(Ebeling+Kalita, 2019)
Write:	<<[EK2019] A1758N JFG1>> <<[EK2019] JHHMMSS.sss+DDMMSS.ss>>
N:	1+66
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST ACS and Keck-II DEIMOS observations of N=1 jellyfish galaxy and N=66 galaxies in the field of the two components, A1758S and A1758N, of the galaxy cluster Abell 1758.
in source:	ACO 1758
Ref:	=2019ApJ...882..127E
by	EBELING H. , KALITA B.S.
	Astrophys. J., 882, 127-127 (2019)
	Jellyfish: ram pressure stripping as a diagnostic tool in studies of cluster collisions.
o	<[EK2019] A1758N JFG1> N=1. Table 2: <[EK2019] JHHMMSS.sss+DDMMSS.ss> N=66.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EKB2017]
[EKB2017]	(Evans+Kennea+Barthelmy+, 2017)
Write:	<<[EKB2017] Source N>>
N:	7
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Swift XRT observations of N=7 X-ray sources, as potential counterparts to a Fermi LAT source in the error region of GrW 170608.
Ref:	=2017GCN.21233....1E
Auth.:	EVANS P.A.+
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EKB95]
[EKB95]	(Elmegreen+Kaufman+Brinks+, 1995)
Write:	<<[EKB95] IN>> <<[EKB95] NN>>
N:	5+6
Object:	HI giant Cloud (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	N=5 clouds in IC 2463, (Nos I1-I5). N=6 clouds in NGC 2207, (Nos N1-N6). See also [EKS2000], [EKE2001]. See also [KBE97] in NGC 2535.
in source:	IC 2463
in source:	NGC 2207
Ref:	=1995ApJ...453..100E
by	ELMEGREEN D.M. , KAUFMAN M., BRINKS E., ELMEGREEN B.G., SUNDIN M.
	Astrophys. J., 453, 100-138 (1995)
	The interaction between spiral galaxies IC 2163 and NGC 2207. I. Observations.
o	Table 6: <[EKB95] AN> (Nos I1-I5) and (Nos N1-N6)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EKE2001]
[EKE2001]	(Elmegreen+Kaufman+Elmegreen+, 2001)= (SSC)
Write:	<<[EKE2001] NN>>
N:	17
Object:	Super Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST observations. N=17 super star clusters in IC 2163 and its companion NGC 2207. See also [EKB95], [EKS2000].
in source:	IC 2163
in source:	NGC 2207
Ref:	=2001AJ....121..182E
by	ELMEGREEN D.M. , KAUFMAN M., ELMEGREEN B.G., BRINKS E., STRUCK C., KLARIC M., THOMASSON M.
	Astron. J., 121, 182-197 (2001)
	Hubble space telescope observations of dust and star-forming regions in the ocular galaxy IC 2163 and its spiral companion NGC 2207.
o	Fig.12, Table 2: <[EKE2001] NN> (Nos 1-17).
=E=	Catalogue in electronic form as J/AJ/121/182
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EKG2019]
[EKG2019]	(Escala+Kirby+Gilbert+, 2019)
Write:	<<[EKG2019] NNNNNNN>>
N:	11
Object:	RGB* (SIMBAD class: RGB* = Red Giant Branch star)
Note:	Keck DEIMOS observations of N=11 red giant branch (RGB) stars in the smooth halo of M31. See also [GKE2019], [EGK2020], and [EKG2020].
in source:	NGC 224 = M 31
Ref:	=2019ApJ...878...42E
by	ESCALA I. , KIRBY E.N., GILBERT K.M., CUNNINGHAM E.C., WOJNO J.
	Astrophys. J., 878, 42-42 (2019)
	Elemental abundances in M31: α and iron element abundances from low-resolution resolved stellar spectroscopy in the stellar halo.
o	Table 8: <[EKG2019] NNNNNNN> N=11 among (Nos 1282178-1303502).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EKG2020]
[EKG2020]	(Escala+Kirby E.n.+Gilbert+, 2020)
Write:	<<[EKG2020] NNNNNNN>>
N:	205
Object:	RGB* (SIMBAD class: RGB* = Red Giant Branch star)
Stat:	is completely incorporated in Simbad
Note:	Keck DEIMOS observations of N=205 red giant branch stars (RGB) in the stellar halo of M 31. See also [GKE2019], [EKG2019] and [EGK2020].
in source:	NGC 224 = M 31
Ref:	=2020ApJ...902...51E
by	ESCALA I. , KIRBY E.N., GILBERT K.M., WOJNO J., CUNNINGHAM E.C., GUHATHAKURTA P.
	Astrophys. J., 902, 51-51 (2020)
	Elemental abundances in M31: properties of the inner stellar halo.
o	Table 4: <[EKG2020] NNNNNNN> N=205 among (Nos 1092174-8005126).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EKH2004]
[EKH2004]	(Edmonds+Kahabka+Heinke, 2004)
Write:	<<[EKH2004] Star A>>
N:	2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Use of archival HST data to identify an optical counterpart to 1E 1339.8+2837: 2 stars are found in the error circle of the X-ray source, Star A is almost certainly the optical counterpart of 1E 1339.8+2837.
in source:	M 3 = NGC 5272
Ref:	=2004ApJ...611..413E
by	EDMONDS P.D. , KAHABKA P., HEINKE C.O.
	Astrophys. J., 611, 413-417 (2004)
	Hubble space telescope discovery of an optical counterpart to the supersoft X-ray source in the globular cluster M3.
o	Figs: <[EKH2004] Star A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EKM99]
[EKM99]	(Evans+Kim+Mazzarella+, 1999)
Write:	<<[EKM99] PKS 1345+12 WW>>
N:	2
Object:	Nuclei (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST NICMOS and OVRO millimeter array observations of the rG PKS 1345+12: N=2 nuclei, SE and NW of the rG.
in source:	PKS 1345+125 = 1Jy 1345+125
Ref:	=1999ApJ...521L.107E
by	EVANS A.S. , KIM D.C., MAZZARELLA J.M., SCOVILLE N.Z., SANDERS D.B.
	Astrophys. J., 521, 107-110 (1999)
	Molecular gas in the powerful radio nucleus of the ultraluminous infrared galaxy PKS 1345+12.
o	Table 1: <[EKM99] PKS 1345+12 WW> (Nos SE, NW).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EKN84]
[EKN84]	(Egikian+Kalloghlian+Nanni+, 1984)
Write:	<<[EKN84] NNN>>
N:	395
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	See also: [KEN83], [VTN88]
in source:	ACO 1213
Ref:	=1984Afz....21...21E
by	EGIKIAN A.G. , KALLOGHLIAN A.T., NANNI D., TREVESE D., VIGNATO A.
	Astrofizika, 21, 21-34 (1984)
	Two-colour photometry of clusters of galaxies. II. A 1213.
o	Table 1: <[EKN84] NNN> (Nos 1-395)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EKP2016]
[EKP2016]	(Evans+Kennea+Palmer+, 2016)
Write:	<<[EKP2016] JHHMMSS.ss+DDMMSS.s>>
N:	16
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Swift XRT observations of N=16 X-ray sources, possible counterparts of the gravitational wave event GW151226.
Ref:	=2016MNRAS.462.1591E
by	EVANS P.A. , KENNEA J.A., PALMER D.M., BILICKI M., OSBORNE J.P., O'BRIEN P.T., TANVIR N.R., LIEN A.Y., BARTHELMY S.D., BURROWS D.N., CAMPANA S., CENKO S.B., D'ELIA V., GEHRELS N., MARSHALL F.E., PAGE K.L., PERRI M., SBARUFATTI B., SIEGEL M.H., TAGLIAFERRI G., TROJA E.
	Mon. Not. R. Astron. Soc., 462, 1591-1602 (2016)
	Swift follow-up of gravitational wave triggers: results from the first aLIGO run and optimization for the future.
o	The trigger G194575 is not in Simbad. Table 3: 2RXP J123044.7+122331 does not exist in the 2RXP catalog.
o	(Erratum) erratum vol. 484, p. 2362 (2019)
o	Table 3: <[EKP2016] JHHMMSS.ss+DDMMSS.s> N=16.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EKS2000]
[EKS2000]	(Elmegreen+Kaufman+Struck+, 2000)
Write:	<<[EKS2000] a>>
N:	21
Object:	Feature (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST WFPC2 observations of peculiar features in the interacting galaxies NGC 2207 and IC 2163. See also [EKB95], [EKE2001], [EEK2006].
in source:	NGC 2207
in source:	IC 2163
Ref:	=2000AJ....120..630E
by	ELMEGREEN B.G. , KAUFMAN M., STRUCK C., ELMEGREEN D.M., BRINKS E., THOMASSON M., KLARIC M., LEVAY Z., ENGLISH J., FRATTARE L.M., BOND H.E., CHRISTIAN C.A., HAMILTON F., NOLL K.
	Astron. J., 120, 630-644 (2000)
	Hubble space telescope observations of the interacting galaxies NGC 2207 and IC 2163.
o	(Erratum) Erratum vol. 120, p. 3371 (2000)
o	Figs 6-7: <[EKS2000] a> (Nos a-u).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EKS96]
[EKS96]	(Evans+Koratkar+Storchi-Bergmann+, 1996)
Write:	<<[EKS96] NGC NNNN NNN>>
N:	2608
Object:	HII (SIMBAD class: HIIReg = HII Region)
in source:	NGC 788
in source:	NGC 1068
in source:	NGC 1097
in source:	NGC 1672
in source:	NGC 2782
in source:	NGC 3081
in source:	NGC 4051
in source:	NGC 4593
in source:	NGC 4639
in source:	NGC 4939
in source:	NGC 5033
in source:	NGC 5427
in source:	NGC 6300
in source:	NGC 6814
in source:	NGC 7213
in source:	NGC 7314
in source:	NGC 7469
Ref:	=1996ApJS..105...93E
by	EVANS I.N. , KORATKAR A.P., STORCHI-BERGMANN T., KIRKPATRICK H., HECKMAN T.M., WILSON A.S.
	Astrophys. J., Suppl. Ser., 105, 93-127 (1996)
	An atlas of H II regions in nearby Seyfert galaxies.
o	Table 2: <[EKS96] NGC NNNN NNN> N=2608
=E=	Catalogue in electronic form as J/ApJS/105/93
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EL
EL	(Eggen+Lynga)
*****	Avoid the usage of EL, prefer [EL68]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: El
El	(Elias)
Note:	Often used for Elias 2- stars
*****	Avoid the usage of El, prefer Elia
Details on Acronym: [EL2001]
[EL2001]	(Ellison+Lopez, 2001)
Write:	<<[EL2001] DLA A>> <<[EL2001] DLA A N>> <<[EL2001] QSO J2316-4041 abs N.NNNN>> <<[EL2001] QSO J2316-4041 abs N.NNNNNN>>
N:	2+5
Object:	DLA
Note:	UVES VLT observations. N=2 DLAs A and B in the line of sight of QSO J2316-4041. The two absorption line systems have been discoved in the CORALS survey (see also [EYH2001]). DLA A is composed of one cloud 'DLA A 1', DLA B is divided in 4 clouds 1 to 4.
Ref:	=2001A&A...380..117E
by	ELLISON S.L. , LOPEZ S.
	Astron. Astrophys., 380, 117-122 (2001)
	Unusual metal abundances in a pair of damped Lyman α systems at z~2.
o	(Erratum) Erratum vol. 392, p. 489 (2002)
o	Text, Table 1: <[EL2001] DLA A> (Nos A-B) = <[EL2001] QSO J2316-4041 abs N.NNNN> N=2, <[EL2001] DLA A N> (No. 1) = <[EL2001] QSO J2316-4041 abs N.NNNNNN> N=1, <[EL2001] DLA B N> (Nos 1-4) = <[EL2001] QSO J2316-4041 abs N.NNNNNN> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EL68]
[EL68]	(Eggen+Lynga, 1968)= (EL)
Write:	<<[EL68] NN>>
N:	7
Object:	Blue * (SIMBAD class: Star)
Note:	Blue stars near Cen X-2 source.
Ref:	=1968ApJ...153L.195E
by	EGGEN O.J. , LYNGA G.
	Astrophys. J., 153, 195-197 (1968)
	Blue objects near Cen X-2.
o	Table 1: <[EL68] NN> N=7 among N>62
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ELAIS
ELAIS	(European Large Area ISO Survey)
Write:	<<ELAIS WN>> <<ELAIS XN>> <<ELAIS aN>> <<ELAIS bN>>
N:	5+6+4
Object:	Field (SIMBAD class: Region = Region defined in the Sky)
Stat:	is completely incorporated in Simbad
Note:	ELAIS survey main fields.
Ref:	=2000MNRAS.316..749O
by	OLIVER S. , ROWAN-ROBINSON M., ALEXANDER D.M., ALMAINI O., BALCELLS M., BAKER A.C., BARCONS X., BARDEN M., BELLAS-VELIDIS I., CABRERA-GUERRA F., CARBALLO R., CESARSKY C.J., CILIEGI P., CLEMENTS D.L., CROCKETT H., DANESE L., DAPERGOLAS A., DROLIAS B., EATON N., EFSTATHIOU A., EGAMI E., ELBAZ D., FADDA D., FOX M., FRANCESCHINI A., GENZEL R., GOLDSCHMIDT P., GRAHAM M., GONZALEZ-SERRANO J.I., GONZALEZ-SOLARES E.A., GRANATO G.L., GRUPPIONI C., HERBSTMEIER U., HERAUDEAU P., JOSHI M., KONTIZAS E., KONTIZAS M., KOTILAINEN J.K., KUNZE D., LA FRANCA F., LARI C., LAWRENCE A., LEMKE D., LINDEN-VORNLE M.J.D., MANN R.G., MARQUEZ I., MASEGOSA J., MATTILA K., McMAHON R.G., MILEY G., MISSOULIS V., MOBASHER B., MOREL T., NORGAARD-NIELSEN H., OMONT A., PAPADOPOULOS P., PEREZ-FOURNON I., PUGET J.-L., RIGOPOULOU D., ROCCA-VOLMERANGE B., SERJEANT S., SILVA L., SUMNER T., SURACE C., VAISANEN P., VAN DER WERF P.P., VERMA A., VIGROUX L., VILLAR-MARTIN M., WILLOTT C.J.
	Mon. Not. R. Astron. Soc., 316, 749-767 (2000)
	The European Large Area ISO Survey - I. Goals, definition and observations.
o	Table 3: <ELAIS WN> (Nos N1-N3, S1-S2), <ELAIS AN> (Nos X1-X6).
Ref:	=2001A&A...379..798P
by	PASCUAL S. , GALLEGO J., ARAGON-SALAMANCA A., ZAMORANO J.
	Astron. Astrophys., 379, 798-806 (2001)
	Hα emitting galaxies and the star formation rate density at z ≃ 0.24.
o	Table 1: <ELAIS aN> (Nos a3-a4, b3-b4). Tables 2: <[PGA2001] ELAIS aN NNNNN> N=25+19+5+20.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: ELAIS
ELAIS	(European Large Area ISO Survey)
*****	Avoid the usage of ELAIS, prefer [PGA2001]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ELAISC15
ELAISC15	(European Large Area ISO Survey, Camera selected at 15 mu.m)
Write:	<<ELAISC15 JHHMMSS+DDMMSS>>
N:	about 2000
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	ELAIS Survey at 15 mu.m.
Ref:	=2001MNRAS.325.1173L
by	LARI C. , POZZI F., GRUPPIONI C., AUSSEL H., CILIEGI P., DANESE L., FRANCESCHINI A., OLIVER S., ROWAN-ROBINSON M., SERJEANT S.
	Mon. Not. R. Astron. Soc., 325, 1173-1189 (2001)
	A new method for ISOCAM data reduction - I. Application to the European Large Area ISO Survey Southern Field: method and results.
o	Tables 5, 6: <ELAISC15 JHHMMSS+DDMMSS> N=456.
Ref:	=2004MNRAS.351.1290R
by	ROWAN-ROBINSON M. , LARI C., PEREZ-FOURNON I., GONZALEZ-SOLARES E.A., LA FRANCA F., VACCARI M., OLIVER S., GRUPPIONI C., CILIEGI P., HERAUDEAU P., SERJEANT S., EFSTATHIOU A., BABBEDGE T., MATUTE I., POZZI F., FRANCESCHINI A., VAISANEN P., AFONSO-LUIS A., ALEXANDER D.M., ALMAINI O., BAKER A.C., BASILAKOS S., BARDEN M., DEL BURGO C., BELLAS-VELIDIS I., CABRERA-GUERRA F., CARBALLO R., CESARSKY C.J., CLEMENTS D.L., CROCKETT H., DANESE L., DAPERGOLAS A., DROLIAS B., EATON N., EGAMI E., ELBAZ D., FADDA D., FOX M., GENZEL R., GOLDSCHMIDT P., GONZALEZ-SERRANO J.I., GRAHAM M., GRANATO G.L., HATZIMINAOGLOU E., HERBSTMEIER U., JOSHI M., KONTIZAS E., KONTIZAS M., KOTILAINEN J.K., KUNZE D., LAWRENCE A., LEMKE D., LINDEN-VORNLE M.J.D., MANN R.G., MARQUEZ I., MASEGOSA J., McMAHON R.G., MILEY G., MISSOULIS V., MOBASHER B., MOREL T., NORGAARD-NIELSEN H., OMONT A., PAPADOPOULOS P., PUGET J.-L., RIGOPOULOU D., ROCCA-VOLMERANGE B., SEDGWICK N., SILVA L., SUMNER T., SURACE C., VILA-VILARO B., VAN DER WERF P., VERMA A., VIGROUX L., VILLAR-MARTIN M., WILLOTT C.J., CARRAMINANA A., MUJICA R.
	Mon. Not. R. Astron. Soc., 351, 1290-1306 (2004)
	The European Large-Area ISO Survey (ELAIS): the final band-merged catalogue.
o	Catalog: <ELAISC7 JHHMMSS+DDMMSS> N=741, <ELAISC15 JHHMMSS+DDMMSS> N=1636, <ELAISR JHHMMSS+DDMMSS> N=1136, <ELAISP90 JHHMMSS+DDMMSS> N=239.
Ref:	=2005MNRAS.358..333G
by	GONZALEZ-SOLARES E.A. , PEREZ-FOURNON I., ROWAN-ROBINSON M., OLIVER S., VACCARI M., LARI C., IRWIN M., McMAHON R.G., HODGKIN S., CILIEGI P., SERJEANT S., WILLOTT C.J.
	Mon. Not. R. Astron. Soc., 358, 333-340 (2005)
	The European Large Area ISO Survey: optical identifications of 15-µm and 1.4-GHz sources in N1 and N2.
o	Table 1: <ELAISC15 JHHMMSS+DDMMSS> N=1172. Table 2: <ELAISR JHHMMSS+DDMMSSA> N=706.
=E=	Catalogue in electronic form as J/MNRAS/325/1173
=E=	Catalogue in electronic form as J/MNRAS/351/1290
=E=	Catalogue in electronic form as J/MNRAS/358/333
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: ELAISC7
ELAISC7	(European Large Area ISO Survey, Camera selected at 6.7 mu.m)
Write:	<<ELAISC7 JHHMMSS+DDMMSS>>
N:	741
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	ELAIS Survey at 6.7 mu.m.
Ref:	=2004MNRAS.351.1290R
by	ROWAN-ROBINSON M. , LARI C., PEREZ-FOURNON I., GONZALEZ-SOLARES E.A., LA FRANCA F., VACCARI M., OLIVER S., GRUPPIONI C., CILIEGI P., HERAUDEAU P., SERJEANT S., EFSTATHIOU A., BABBEDGE T., MATUTE I., POZZI F., FRANCESCHINI A., VAISANEN P., AFONSO-LUIS A., ALEXANDER D.M., ALMAINI O., BAKER A.C., BASILAKOS S., BARDEN M., DEL BURGO C., BELLAS-VELIDIS I., CABRERA-GUERRA F., CARBALLO R., CESARSKY C.J., CLEMENTS D.L., CROCKETT H., DANESE L., DAPERGOLAS A., DROLIAS B., EATON N., EGAMI E., ELBAZ D., FADDA D., FOX M., GENZEL R., GOLDSCHMIDT P., GONZALEZ-SERRANO J.I., GRAHAM M., GRANATO G.L., HATZIMINAOGLOU E., HERBSTMEIER U., JOSHI M., KONTIZAS E., KONTIZAS M., KOTILAINEN J.K., KUNZE D., LAWRENCE A., LEMKE D., LINDEN-VORNLE M.J.D., MANN R.G., MARQUEZ I., MASEGOSA J., McMAHON R.G., MILEY G., MISSOULIS V., MOBASHER B., MOREL T., NORGAARD-NIELSEN H., OMONT A., PAPADOPOULOS P., PUGET J.-L., RIGOPOULOU D., ROCCA-VOLMERANGE B., SEDGWICK N., SILVA L., SUMNER T., SURACE C., VILA-VILARO B., VAN DER WERF P., VERMA A., VIGROUX L., VILLAR-MARTIN M., WILLOTT C.J., CARRAMINANA A., MUJICA R.
	Mon. Not. R. Astron. Soc., 351, 1290-1306 (2004)
	The European Large-Area ISO Survey (ELAIS): the final band-merged catalogue.
o	Catalog: <ELAISC7 JHHMMSS+DDMMSS> N=741, <ELAISC15 JHHMMSS+DDMMSS> N=1636, <ELAISR JHHMMSS+DDMMSS> N=1136, <ELAISP90 JHHMMSS+DDMMSS> N=239.
=E=	Catalogue in electronic form as J/MNRAS/351/1290
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ELAISP90
ELAISP90	(European Large Area ISO Survey, Preliminary 90 mu.m)
Write:	<<ELAISP90 JHHMMSS+DDMMSS>>
N:	38+239
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	ELAIS Survey. preliminary results at 90mu.m
Ref:	=2001MNRAS.322..262S
by	SERJEANT S. , EFSTATHIOU A., OLIVER S., SURACE C., HERAUDEAU P., LINDEN-VORNLE M.J.D., GRUPPIONI C., LA FRANCA F., RIGOPOULOU D., MOREL T., CROCKETT H., SUMNER T., ROWAN-ROBINSON M., GRAHAM M.
	Mon. Not. R. Astron. Soc., 322, 262-268 (2001)
	The European Large Area ISO Survey - IV. The preliminary 90-µm luminosity function.
o	Table 1: <ELAISP90 JHHMMSS+DDMMSS> N=38.
Ref:	=2004MNRAS.351.1290R
by	ROWAN-ROBINSON M. , LARI C., PEREZ-FOURNON I., GONZALEZ-SOLARES E.A., LA FRANCA F., VACCARI M., OLIVER S., GRUPPIONI C., CILIEGI P., HERAUDEAU P., SERJEANT S., EFSTATHIOU A., BABBEDGE T., MATUTE I., POZZI F., FRANCESCHINI A., VAISANEN P., AFONSO-LUIS A., ALEXANDER D.M., ALMAINI O., BAKER A.C., BASILAKOS S., BARDEN M., DEL BURGO C., BELLAS-VELIDIS I., CABRERA-GUERRA F., CARBALLO R., CESARSKY C.J., CLEMENTS D.L., CROCKETT H., DANESE L., DAPERGOLAS A., DROLIAS B., EATON N., EGAMI E., ELBAZ D., FADDA D., FOX M., GENZEL R., GOLDSCHMIDT P., GONZALEZ-SERRANO J.I., GRAHAM M., GRANATO G.L., HATZIMINAOGLOU E., HERBSTMEIER U., JOSHI M., KONTIZAS E., KONTIZAS M., KOTILAINEN J.K., KUNZE D., LAWRENCE A., LEMKE D., LINDEN-VORNLE M.J.D., MANN R.G., MARQUEZ I., MASEGOSA J., McMAHON R.G., MILEY G., MISSOULIS V., MOBASHER B., MOREL T., NORGAARD-NIELSEN H., OMONT A., PAPADOPOULOS P., PUGET J.-L., RIGOPOULOU D., ROCCA-VOLMERANGE B., SEDGWICK N., SILVA L., SUMNER T., SURACE C., VILA-VILARO B., VAN DER WERF P., VERMA A., VIGROUX L., VILLAR-MARTIN M., WILLOTT C.J., CARRAMINANA A., MUJICA R.
	Mon. Not. R. Astron. Soc., 351, 1290-1306 (2004)
	The European Large-Area ISO Survey (ELAIS): the final band-merged catalogue.
o	Catalog: <ELAISC7 JHHMMSS+DDMMSS> N=741, <ELAISC15 JHHMMSS+DDMMSS> N=1636, <ELAISR JHHMMSS+DDMMSS> N=1136, <ELAISP90 JHHMMSS+DDMMSS> N=239.
=E=	Catalogue in electronic form as J/MNRAS/351/1290
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ELAISR
ELAISR	(European Large-Area ISO Survey, Radio catalogue)= (ELAISR20)
Write:	<<ELAISR JHHMMSS+DDMMSSA>>
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ELAIS Survey, radio selected sources. The different components of multiple sources are labeled A, B, ... 1999MNRAS.302..222C: Northern ELAIS fields (VLA survey). 1999MNRAS.305..297G: Southern ELAIS field (ATCA survey).
Ref:	=1999MNRAS.302..222C
by	CILIEGI P. , McMAHON R.G., MILEY G., GRUPPIONI C., ROWAN-ROBINSON M., CESARSKY C., DANESE L., FRANCESCHINI A., GENZEL R., LAWRENCE A., LEMKE D., OLIVER S., PUGET J.-L., ROCCA-VOLMERANGE B.
	Mon. Not. R. Astron. Soc., 302, 222-244 (1999)
	A deep VLA survey at 20 cm of the ISO ELAIS survey regions.
o	Table 3: <ELAISR JHHMMSS+DDMMSSA> N=964.
Ref:	=1999MNRAS.305..297G
by	GRUPPIONI C. , CILIEGI P., ROWAN-ROBINSON M., CRAM L., HOPKINS A., CESARSKY C., DANESE L., FRANCESCHINI A., GENZEL R., LAWRENCE A., LEMKE D., McMAHON R.G., MILEY G., OLIVER S., PUGET J.-L., ROCCA-VOLMERANGE B.
	Mon. Not. R. Astron. Soc., 305, 297-308 (1999)
	A 1.4-GHz survey of the southern European Large-Area ISO Survey region.
o	Table 1: <ELAISR JHHMMSS+DDMMSSA> N=650.
Ref:	=2004MNRAS.351.1290R
by	ROWAN-ROBINSON M. , LARI C., PEREZ-FOURNON I., GONZALEZ-SOLARES E.A., LA FRANCA F., VACCARI M., OLIVER S., GRUPPIONI C., CILIEGI P., HERAUDEAU P., SERJEANT S., EFSTATHIOU A., BABBEDGE T., MATUTE I., POZZI F., FRANCESCHINI A., VAISANEN P., AFONSO-LUIS A., ALEXANDER D.M., ALMAINI O., BAKER A.C., BASILAKOS S., BARDEN M., DEL BURGO C., BELLAS-VELIDIS I., CABRERA-GUERRA F., CARBALLO R., CESARSKY C.J., CLEMENTS D.L., CROCKETT H., DANESE L., DAPERGOLAS A., DROLIAS B., EATON N., EGAMI E., ELBAZ D., FADDA D., FOX M., GENZEL R., GOLDSCHMIDT P., GONZALEZ-SERRANO J.I., GRAHAM M., GRANATO G.L., HATZIMINAOGLOU E., HERBSTMEIER U., JOSHI M., KONTIZAS E., KONTIZAS M., KOTILAINEN J.K., KUNZE D., LAWRENCE A., LEMKE D., LINDEN-VORNLE M.J.D., MANN R.G., MARQUEZ I., MASEGOSA J., McMAHON R.G., MILEY G., MISSOULIS V., MOBASHER B., MOREL T., NORGAARD-NIELSEN H., OMONT A., PAPADOPOULOS P., PUGET J.-L., RIGOPOULOU D., ROCCA-VOLMERANGE B., SEDGWICK N., SILVA L., SUMNER T., SURACE C., VILA-VILARO B., VAN DER WERF P., VERMA A., VIGROUX L., VILLAR-MARTIN M., WILLOTT C.J., CARRAMINANA A., MUJICA R.
	Mon. Not. R. Astron. Soc., 351, 1290-1306 (2004)
	The European Large-Area ISO Survey (ELAIS): the final band-merged catalogue.
o	Catalog: <ELAISC7 JHHMMSS+DDMMSS> N=741, <ELAISC15 JHHMMSS+DDMMSS> N=1636, <ELAISR JHHMMSS+DDMMSS> N=1136, <ELAISP90 JHHMMSS+DDMMSS> N=239.
Ref:	=2005MNRAS.358..333G
by	GONZALEZ-SOLARES E.A. , PEREZ-FOURNON I., ROWAN-ROBINSON M., OLIVER S., VACCARI M., LARI C., IRWIN M., McMAHON R.G., HODGKIN S., CILIEGI P., SERJEANT S., WILLOTT C.J.
	Mon. Not. R. Astron. Soc., 358, 333-340 (2005)
	The European Large Area ISO Survey: optical identifications of 15-µm and 1.4-GHz sources in N1 and N2.
o	Table 1: <ELAISC15 JHHMMSS+DDMMSS> N=1172. Table 2: <ELAISR JHHMMSS+DDMMSSA> N=706.
=E=	Catalogue in electronic form as J/MNRAS/302/222
=E=	Catalogue in electronic form as J/MNRAS/305/297
=E=	Catalogue in electronic form as J/MNRAS/351/1290
=E=	Catalogue in electronic form as J/MNRAS/358/333
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ELAISR20
ELAISR20	(European Large-Area ISO Survey, Radio catalogue at 20cm)
*****	Avoid the usage of ELAISR20, prefer ELAISR
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ELARS
ELARS	(Extended Lyman Alpha Reference Sample)
Write:	<<ELARS NN>>
N:	28
Object:	Em. G (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	HST observations of N=28 galaxies with extended Lymanα emission. See also LARS.
Ref:	=2023ApJS..266...15M
by	MELINDER J. , OSTLIN G., HAYES M., RASEKH A., MAS-HESSE J.M., CANNON J.M., KUNTH D., LAURSEN P., RUNNHOLM A., HERENZ E.C., MESSA M., SCHAERER D., VERHAMME A., RIVERA-THORSEN T.E., GUAITA L., MARQUART T., PUSCHNIG J., LE RESTE A., SANDBERG A., FREELAND E., BRIDGE J.
	Astrophys. J., Suppl. Ser., 266, 15 (2023)
	The Lyα Reference Sample. XIV. Lyα Imaging of 45 Low-redshift Star-forming Galaxies and Inferences on Global Emission.
o	Figs 3-5, Table 1: <ELARS NN> (Nos 01-28).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ELC2017]
[ELC2017]	(Eswaraiah+Lai+Chen+, 2017)
Write:	<<[ELC2017] NNNN>>
N:	1074
Object:	* (SIMBAD class: Star)
Note:	SAAO IRSF 1.4m telescope SIRPOL photometric observations of N=1074 stars in the central star-forming region of RCW 57A.
in source:	RCW 57A = NGC 3576
Ref:	=2017ApJ...850..195E
by	ESWARAIAH C. , LAI S.-P., CHEN W.-P., PANDEY A.K., TAMURA M., MAHESWAR G., SHARMA S., WANG J.-W., NISHIYAMA S., NAKAJIMA Y., KWON J., PURCELL R., MAGALHAES A.M.
	Astrophys. J., 850, 195-195 (2017)
	Understanding the links among the magnetic fields, filament, bipolar bubble, and star formation in RCW 57A using NIR polarimetry.
o	Table 1: <[ELC2017] NNNN> (Nos 1-1074).
=E=	Catalogue in electronic form as J/ApJ/850/195
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ELG88]
[ELG88]	(Eiroa+Lenzen+Gomez, 1988)
Write:	<<[ELG88] INa>>
N:	9
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	* around [WBN74] NGC 7538 IRS 9
Ref:	=1988A&A...190..283E
by	EIROA C. , LENZEN R., GOMEZ A.I.
	Astron. Astrophys., 190, 283-288 (1988)
	The nature of the reflection nebula associated with NGC 7538/IRS 9.
o	IRS 9 = [WBN74] NGC 7538 IRS 9
o	Table 1: <[ELG88] INa> (Nos I1a-I1b, I2-I3, I4a-I4b, I5-I7)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ELG99]
[ELG99]	(Eales+Lilly+Gear+, 1999)= (CFRS)
Write:	<<[ELG99] CFRS HHA>>
N:	12
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SCUBA observations of CFRS fields: detection of 12 sources at 850mu.m. In the format, 'HH' stands for hours of R.A.. See also CUDSS, [FHD99].
Ref:	=1999ApJ...515..518E
by	EALES S. , LILLY S., GEAR W., DUNNE L., BOND J.R., HAMMER F., LE FEVRE O., CRAMPTON D.
	Astrophys. J., 515, 518-524 (1999)
	The Canada-UK deep submillimeter survey: first submillimeter images, the source counts, and resolution of the background.
o	Table 1: <[ELG99] CFRS HHA> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ELH2006]
[ELH2006]	(Erdogdu+Lahav+Huchra+, 2006)
Write:	<<[ELH2006] VNN>> <<[ELH2006] CNN>>
N:	15+33
Object:	Void + Cluster of G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Overdensities (CNN) and voids (VNN) in the 2MRS density field.
Ref:	=2006MNRAS.373...45E
by	ERDOGDU P. , LAHAV O., HUCHRA J.P., COLLESS M., CUTRI R.M., FALCO E., GEORGE T., JARRETT T., JONES D.H., MACRI L.M., MADER J., MARTIMBEAU N., PAHRE M.A., PARKER Q.A., RASSAT A., SAUNDERS W.
	Mon. Not. R. Astron. Soc., 373, 45-64 (2006)
	Reconstructed density and velocity fields from the 2MASS Redshift Survey.
o	Paragr. 6.1: <[ELH2006] VNN> (Nos V1-V15), <[ELH2006] CNN> (Nos C1-C33).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ELHC
ELHC	(EROS, LMC, HAeBe Candidate)= (EROS ELHC)
Write:	<<ELHC NN>>
N:	21
Object:	PMS* (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	EROS 2 LMC observations. See also ESHC.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1996Sci...272..995B
by	BEAULIEU J.P. , LAMERS H.J.G.L.M., GRISON P., JULIEN R., LANCIAUX C., FERLET R., VIDAL-MADJAR A., BERTIN E., MAURICE E., PREVOT L., GRY C., GUIBERT J., MOREAU O., TAJHMADY F., AUBOURG E., BAREYRE P., DE KAT J., GROS M., LAURENT B., LACHIEZE-REY M., LESQUOY E., MAGNEVILLE C., MILSZTAJN A., MOSCOSO L., QUEINNEC F., RENAULT C., RICH J., SPIRO M., VIGROUX L., ZYLBERAJCH S., ANSARI R., CAVALIER F., MONIEZ M.
	Science, 272, 995-997 (1996)
	Pre-main-sequence star candidates in the bar of the Large Magellanic Cloud.
o	Table 1: <ELHC N> (Nos 1-7)
Ref:	=2002A&A...395..829D
by	DE WIT W.J. , BEAULIEU J.P., LAMERS H.J.G.L.M.
	Astron. Astrophys., 395, 829-844 (2002)
	A Search for HAeBe stars in the bar of the Large Magellanic Cloud based on optical variability.
o	Table 1, A1: <ELHC NN> (Nos 8-21) added.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ELHS
ELHS	(Erroneous Luyten, Half Second) (Not yet in Simbad)
Write:	<<ELHS NNNN>>
N:	2
Object:	* (SIMBAD class: HighPM* = High Proper Motion Star)
Note:	Two stars have mistaken indentities: LHS 2067 and LHS 2068, they are named ELHS 2067 and ELHS 2068 by the authors (E for Erroneous), and new LHS 2067 and LHS 2068 are introduced.
Ref:	=1995PASP..107..742M
by	MULLIS C.R. , BEGAM M.C., IANNA P.A.
	Publ. Astron. Soc. Pac., 107, 742-743 (1995)
	The mistaken identities of LHS 2067 and LHS 2068.
o	ELHS 2067 and 2068 = Erroneous LHS stars, not in SIMBAD. New LHS 2067 and LHS 2068 are introduced.
o	<ELHS NNNN> (Nos 2067, 2068).
Details on Acronym: Elia
Elia	(Elias)= (El) = Elias = (Oph)
Write:	<<Elia 1-NN>> <<Elia 2-NN>> <<Elia 3-NN>>
N:	16+87+30
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	In IC 5146: (Nos 1-16), format '1-NN'. In ρ Oph: (Nos 1-87), format '2-NN'. In Taurus Cloud: (Nos 1-30), format '3-NN'. 1950 coordinates, No Identif. charts
in source:	IC 5146
in source:	NAME rho Oph Cloud
in source:	NAME TMC
Ref:	=1978ApJ...223..859E
by	ELIAS J.H.
	Astrophys. J., 223, 859-875 (1978)
	A study of the IC 5146 dark cloud complex.
o	Tables 1, 2: <Elia 1-NN> (Nos 1-16)
Ref:	=1978ApJ...224..453E
by	ELIAS J.H.
	Astrophys. J., 224, 453-472 (1978)
	An infrared study of the Ophiuchus dark cloud.
o	Tables 2, 3: <Elia 2-NN> (Nos 1-87)
Ref:	=1978ApJ...224..857E
by	ELIAS J.H.
	Astrophys. J., 224, 857-872 (1978)
	A study of the Taurus dark cloud complex.
o	Table 1: <Elia 3-NN> (Nos 1-30)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Elias
Elias	(Elias)
====>	Equivalent to: Elia
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [ELK2021]
[ELK2021]	(Elias-Chavez+Longinotti+Krongold+, 2021)
Write:	<<[ELK2021] NNN>>
N:	301
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton EPIC and GTC OSIRIS observations of N=301 X-ray sources, as part of the 1.75 Ms Ultra Narrow Deep Field (XMM175UNDF) survey.
Ref:	=2021ApJ...919...18E
by	ELIAS-CHAVEZ M. , LONGINOTTI A.L., KRONGOLD Y., VIGNALI C., NICASTRO F., ROSA-GONZALEZ D., MAYYA Y.D., MATHUR S.
	Astrophys. J., 919, 18-18 (2021)
	X-ray sources in the 1.75 Ms Ultra Narrow Deep Field observed by XMM-Newton.
o	Table 6: <[ELK2021] NNN> (Nos 1-301).
=E=	Catalogue in electronic form as <J/ApJ/919/18/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ELL90]
[ELL90]	(Epchtein+Le Bertre+Lepine, 1990)
Write:	<<[ELL90] NNN>>
N:	249
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Photometry of 249 southern IRAS stars.
Ref:	=1990A&A...227...82E
by	EPCHTEIN N. , LE BERTRE T., LEPINE J.R.D.
	Astron. Astrophys., 227, 82-104 (1990)
	Carbon star envelopes: near-IR photometry, mass loss and evolutionary status of a sample of IRAS stars.
o	Table 1: <[ELL90] NNN> (Nos 1-249).
=E=	Catalogue in electronic form as J/A+A/227/82
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ELM93]
[ELM93]	(Eiroa+Lenzen+Miranda+, 1993)= (IRS)
Write:	<<[ELM93] Star N>> <<[ELM93] HH N>> <<[ELM93] HH 1A>> <<[ELM93] IRS N>>
N:	3+4+8+2
Object:	Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 1: format 'IRS N', N=2. Table 2: format 'Star N', N=3, format 'HH N', N=4. Fig. 2: format 'HH 1A', N=8 (Nos A-H)
in source:	SH 2-140 N
Ref:	=1993AJ....106..613E
by	EIROA C. , LENZEN R., MIRANDA L.F., TORRELLES J.M., ANGLADA G., ESTALELLA R.
	Astron. J., 106, 613-617 (1993)
	Optical and near-infrared observations of S 140N.
o	Table 1: <[ELM93] IRS N> N=2, Table 2: <[ELM93] Star N> N=3, <[ELM93] HH N> N=4, Fig. 2: <[ELM93] HH 1A> N=8 (Nos A-H)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ELO
ELO	(Emission-Line Object)
*****	Avoid the usage of ELO, prefer [SDV2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ELS
ELS	(Emission Line *)
====>	Equivalent to: Kiso
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ELS2006]
[ELS2006]	(Evans+Lennon+Smartt+, 2006)
Write:	<<[ELS2006] N11 NNN>> <<[ELS2006] N11 NNNB>>
N:	124+7
Object:	* (SIMBAD class: Star)
Note:	VLT-FLAMES observations of stars in the field of LHA 120-N 11 in the LMC. In the other fields the objects are designated as Cl* NGC 346 ELS, Cl* NGC 330 ELS and Cl* NGC 2004 ELS.
in source:	Magellanic Clouds:LMC:LHA 120-N 11 = LHA 120-N 11
Ref:	=2006A&A...456..623E
by	EVANS C.J. , LENNON D.J., SMARTT S.J., TRUNDLE C.
	Astron. Astrophys., 456, 623-638 (2006)
	The VLT-FLAMES survey of massive stars: observations centered on the Magellanic Cloud clusters NGC330, NGC346, NGC2004, and the N11 region.
o	(Erratum) erratum vol. 464, p. 289 (2007)
o	Table 4: <Cl* NGC 346 ELS NNN> (Nos 1-116). Table 5: <Cl* NGC 330 ELS NNN> (Nos 1-125). Table 6: <[ELS2006] N11 NNN> (Nos 1-124). Table 7: <Cl* NGC 2004 ELS NNN> (Nos 1-119).
Ref:	=2008A&A...479..541H
by	HUNTER I. , LENNON D.J., DUFTON P.L., TRUNDLE C., SIMON-DIAZ S., SMARTT S.J., RYANS R.S.I., EVANS C.J.
	Astron. Astrophys., 479, 541-555 (2008)
	The VLT-FLAMES survey of massive stars: atmospheric parameters and rotational velocity distributions for B-type stars in the Magellanic Clouds.
o	(Erratum) + corrigendum vol. 530 p. C1 (2011)
o	Secondary objects of tables 3, 4, 5 and 6 not in Simbad.
o	Tables 1, 3: <Cl* NGC 346 ELS NNNB> N=5 added, <Cl* NGC 2004 ELS NNNB> N=1 added. Table 5: <[ELS2006] N11 NNNB> N=7 added.
=E=	Catalogue in electronic form as J/A+A/456/623
=E=	Catalogue in electronic form as J/A+A/479/541
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ELS2020]
[ELS2020]	(Eswaraiah+Li+Samal+, 2020) (Not yet in Simbad)
Write:	<<[ELS2020] Clump N>>
Object:	Clump (SIMBAD class: denseCore = Dense Core)
Note:	JCMT SCUBA-2/POL-2 polarization observations of N=2 clumps in Sh 2-201.
in source:	SH 2-201
Ref:	=2020ApJ...897...90E
by	ESWARAIAH C. , LI D., SAMAL M.R., WANG J.-W., MA Y., LAI S.-P., ZAVAGNO A., CHING T.-C., LIU T., PATTLE K., WARD-THOMPSON D., PANDEY A.K., OJHA D.K.
	Astrophys. J., 897, 90-90 (2020)
	Unveiling the importance of magnetic fields in the evolution of dense clumps formed at the waist of bipolar H II regions: a case study of Sh 2-201 with JCMT SCUBA-2/POL-2.
o	Clumps 1 and 2 of Sh 2-201 are not in SIMBAD.
o	Fig. 2, Table 2: <[ELS2020] Clump N> (Nos 1-2).
=E=	Catalogue in electronic form as <J/ApJ/897/90/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ELT2011]
[ELT2011]	(Einasto+Liivamaegi+Tempel+, 2011) (Not yet in Simbad)
Write:	<<[ELT2011] NN>> <<[ELT2011] DDD+DDD+NNN>>
N:	13
Object:	Supercluster of G (SIMBAD class: SuperClG = Supercluster of Galaxies)
Note:	N=13 superclusters of galaxies in the Sloan Great Wall. In the format DDD+DDD+NNN: DDD+DDD are the integer parts of the equatorial coordinates and NNN is the redshift multiplied by 100. See also [LTS2012].
in source:	NAME THE SLOAN GREAT WALL
Ref:	=2011ApJ...736...51E
by	EINASTO M. , LIIVAMAEGI L.J., TEMPEL E., SAAR E., TAGO E., EINASTO P., ENKVIST I., EINASTO J., MARTINEZ V.J., HEINAMAKI P., NURMI P.
	Astrophys. J., 736, 51 (2011)
	The Sloan Great Wall. Morphology and galaxy content.
o	Table 1, col(1): <[ELT2011] NN> (Nos 1-13) = Table 1, col(3): <[ELT2011] DDD+DDD+NNN> N=13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ELT2012]
[ELT2012]	(Einasto M.+Liivamaegi L.j.+Tempel+, 2014)
Write:	<<[ELT2012] DDD+DDD+NNNN>> <<[ELT2012] NNNN>>
N:	50+50
Object:	Supercluster of G (SIMBAD class: SuperClG = Supercluster of Galaxies)
Note:	N=50 superclusters of galaxies from the SDSS DR8. In the format DDD+DDD+NNNN: DDD+DDD are the integer parts of the equatorial coordinates and NNNN is the redshift multiplied by 1000. See also [EVN2012] for clusters in these superclusters.
Ref:	=2012A&A...542A..36E
by	EINASTO M. , LIIVAMAEGI L.J., TEMPEL E., SAAR E., VENNIK J., NURMI P., GRAMANN M., EINASTO J., TAGO E., HEINAEMAEKI P., AHVENSALMI A., MARTINEZ V.J.
	Astron. Astrophys., 542A, 36-36 (2012)
	Multimodality of rich clusters from the SDSS DR8 within the supercluster-void network.
o	Table 6, col(1): <[ELT2012] DDD+DDD+NNNN> N=50 = Table 1, col(2): <[ELT2012] NNNN> N=50 among (Nos 1-1295).
=E=	Catalogue in electronic form as J/A+A/542/A36
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ELT88]
[ELT88]	(Eder+Lewis+Terzian+, 1988)
Write:	<<[ELT88] HHMMm+DDMMa>> <<[ELT88] HHMMm+DDMMA>>
N:	182+96+132
Object:	Maser (SIMBAD class: Maser)
Note:	Arecibo OH (1612MHz) spectroscopic observations of IRAS sources.
Ref:	=1988ApJS...66..183E
by	EDER J. , LEWIS B.M., TERZIAN Y.
	Astrophys. J., Suppl. Ser., 66, 183-207 (1988)
	New OH/IR stars from color-selected iras sources : 1612 MHz observations.
o	Table 2: <[ELT88] HHMMm+DDMMA>, <[ELT88] HHMMm+DDMMa>, N=182.
Ref:	=1990ApJ...362..634L
by	LEWIS B.M. , EDER J., TERZIAN Y.
	Astrophys. J., 362, 634-651 (1990)
	New OH/IR stars from color-selected IRAS sources. II. An unbiased 1612 MHz survey.
o	Table 1: <[ELT88] HHMMm+DDMMa> N=96 added.
Ref:	=1993ApJS...89..189C
by	CHENGALUR J.N. , LEWIS B.M., EDER J., TERZIAN Y.
	Astrophys. J., Suppl. Ser., 89, 189-210 (1993)
	New OH/IR stars from color-selected IRAS sources. III. A complete survey.
o	Table 1: <[ELT88] HHMMm+DDMMa> N=132 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ELZ2004]
[ELZ2004]	(Erdogdu+Lahav+Zaroubi+, 2004)
Write:	<<[ELZ2004] SCSGP NN>> <<[ELZ2004] SCNGP NN>> <<[ELZ2004] VSGP NN>> <<[ELZ2004] VNGP NN>>
N:	20+20+40+30
Object:	SuperCl of G + Void (SIMBAD class: SuperClG = Supercluster of Galaxies)
Note:	Reconstruction of the underlying density field of the 2dFGRS for the redshift range 0.035<z<0.200. Maps of the density fields in the SGP and NGP. Identifications of Spuperclusters and voids.
in source:	NAME SGP
in source:	NAME NGP
Ref:	=2004MNRAS.352..939E
by	ERDOGDU P. , LAHAV O., ZAROUBI S., EFSTATHIOU G., MOODY S., PEACOCK J.A., COLLESS M., BALDRY I.K., BAUGH C.M., BLAND-HAWTHORN J., BRIDGES T., CANNON R., COLE S., COLLINS C., COUCH W., DALTON G., DE PROPRIS R., DRIVER S.P., ELLIS R.S., FRENK C.S., GLAZEBROOK K., JACKSON C., LEWIS I., LUMSDEN S., MADDOX S., MADGWICK D., NORBERG P., PETERSON B.A., SUTHERLAND W., TAYLOR K.
	Mon. Not. R. Astron. Soc., 352, 939-960 (2004)
	The 2dF Galaxy Redshift Survey: Wiener reconstruction of the cosmic web.
o	Table 1: <[ELZ2004] SCSGP NN> (Nos 1-20), Table 1: <[ELZ2004] SCNGP NN> (Nos 1-20). Table 2: <[ELZ2004] VSGP NN> (Nos 1-40). Table 3: <[ELZ2004] VNGP NN> (Nos 1-30).
=E=	Catalogue in electronic form as J/MNRAS/352/939
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Em
Em	(Emission Obj.) (Not yet in Simbad)
*****	Avoid the usage of Em, prefer [M61b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Em
Em	(Emission obj.)
Write:	<<PN Em N>>
N:	3
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Nos 1,2,5. PK Nomenclature. Other objects are [M61b].
Ref:	=1961PASP...73..264M
by	McCUSKEY S.W.
	Publ. Astron. Soc. Pac., 73, 264-265 (1961)
	Emission objects near Selected Area 158.
o	Table I: <[M61b] N> (Nos 1-7), <PN Em N> (Nos 1, 2, 5)
Details on Acronym: [EM2016]
[EM2016]	(Efremov+Moiseev, 2016)
Write:	<<[EM2016] Red Ellipse>>
N:	1
Object:	Superbubble (SIMBAD class: PartofG = Part of a Galaxy)
Note:	SAO RAS 6m BTA telescope SCORPIO-2 observations of N=1 superbubble in the northern arm of NGC 6946.
in source:	NGC 6946
Ref:	=2016MNRAS.461.2993E
by	EFREMOV Y.N. , MOISEEV A.V.
	Mon. Not. R. Astron. Soc., 461, 2993-3000 (2016)
	Imaging and spectroscopic observations of a strange elliptical bubble in the northern arm of the spiral galaxy NGC 6946.
o	<[EM2016] Red Ellipse> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EM94]
[EM94]	(Eisloffel+Mundt, 1994) (Not yet in Simbad)
Write:	<<[EM94] ANN>> <<[EM94] A>> <<[EM94] HH 46-N>>
N:	69+3+3
Object:	Part of HH (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Tables 1, 3, 4: Condensations in HH 46-47, (Nos A0-A28), (Nos B0-B12), (Nos C1-C7), (Nos D1-D20). Table 2: Knots in HH 46-47, (Nos X-Z). Table 1, Fig.3: Condensations in HH 46, (Nos HH 46-1 to HH 46-3)
in source:	NAME HH 46-47
Ref:	=1994A&A...284..530E
by	EISLOEFFEL J. , MUNDT R.
	Astron. Astrophys., 284, 530-544 (1994)
	Proper motion measurements and high resolution imaging of the HH 46/47 outflow.
o	Tables 1, 3, 4: <[EM94] ANN> (Nos A0-A28, B0-B12, C1-C7, D1-D20). Table 2: <[EM94] A> (Nos X, Y, Z). Table 1, Fig.3: <[EM94] HH 46-N> (Nos HH 46-1 to HH 46-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EM96]
[EM96]	(Escalera+MacGillivray, 1996)
Write:	<<[EM96] OA>> <<[EM96] COS-NNNN>>
N:	3+25+19+267
Object:	Region + super Cl + Cluster of G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 11: N=3 voids, (Nos OA-OC). Table 12: the format 'COS-NNNN' is a numerotation of the authors, where 'COS' stands for Coordinates and Sizes' N=25 very large structures (among which N=6 ultra large) (Nos 0001-0025). N=19 superclusters, (Nos 0101-0119). N=267 cluster-sized structures, (Nos 1001-1267). among which N=134 compact cluster or association, N=91 ClG, and N=42 elongated intermediate structures.
Ref:	=1996A&AS..117..519E
by	ESCALERA E. , MacGILLIVRAY H.T.
	Astron. Astrophys., Suppl. Ser., 117, 519-555 (1996)
	Detection of structures on multiple scales around the South Galactic Pole. A two-dimensional analysis of the COSMOS/UKST Southern Sky Galaxy Catalogue.
o	Table 11: <[EM96] OA> (Nos OA-OC). Table 12: <[EM96] COS-NNNN>, (Nos 0001-0025), (Nos 0101-0119), (Nos 1001-1267)
=E=	Catalogue in electronic form as J/A+AS/117/519
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EM98]
[EM98]	(Eisloffel+Mundt, 1998)
Write:	<<[EM98] DG Tau Knot A>> <<[EM98] DG Tau B cRN>> <<[EM98] DG Tau B Knot AN>> <<[EM98] FS Tau B Knot AN>> <<[EM98] FS Tau B Knot cN>> <<[EM98] FS Tau B WW cavity>> <<[EM98] FS Tau B RN>> <<[EM98] FS Tau B RN>> <<[EM98] CoKu Tau 1 Knot A>>
N:	59
Object:	Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	In DG Tau jet and region: N=4 Knots, format 'DG Tau Knot A', (Nos A-D). See also [MBB87]. In DG Tau B region: N=12 Knots, format 'DG Tau B Knot A' or 'AN'. N=1 compact Reflexion Nebula, format 'DG Tau B cRN'. In FS Tau B region: N=18 Knots, format 'FS Tau B Knot A' or 'AN'. See also [MBB87]. N=2 Cavities, format 'FS Tau B NE cavity' and 'SE'. N=5 Knots in the cavities, format 'DG Tau B cN'. N=1 Reflexion Nebula, format 'FS Tau B RN'. N=3 Reflexion Nebulaes, format 'FS Tau B R1' to 'R3'. See also [MBB87]. In CoKu Tau 1 (= CoKu Tau-Aur Star 1 in SIMBAD) region: N=3 Knots, format 'CoKu Tau 1 Knot A', (Nos A-C)
Ref:	=1998AJ....115.1554E
by	EISLOEFFEL J. , MUNDT R.
	Astron. J., 115, 1554-1575 (1998)
	Imaging and kinematic studies of young stellar object jets in Taurus.
o	<HH NNN> (Nos 159, 276). Table 3: <[EM98] DG Tau Knot A> (Nos A-D). Text, Fig.: <[EM98] DG Tau B cRN>. Table 5: <[EM98] DG Tau B Knot AN> (Nos A1-A3, B1-B2, C, D1-D2, F1-F2, G, H). Text, Fig.: <[EM98] FS Tau B Knot AN> (Nos A1-A7, B-L), <[EM98] FS Tau B Knot cN> (Nos c1-c5), <[EM98] FS Tau B WW cavity> (Nos NE, SE), <[EM98] FS Tau B AA> (No. RN) N=1, <[EM98] FS Tau B RN> (Nos R1-R3). Table 9, Fig.: <[EM98] CoKu Tau 1 Knot A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EM99]
[EM99]	(Esteban+Mendez, 1999)
Write:	<<[EM99] NN>> <<[EM99] A>>
N:	20+5
Object:	Knot + Region (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Table 2, Fig.1: N=20 knots in Mrk 8. Fig.4: N=5 regions in Mrk 8, each corresponding to one or several of the knots.
in source:	Mrk 8
Ref:	=1999A&A...348..446E
by	ESTEBAN C. , MENDEZ D.I.
	Astron. Astrophys., 348, 446-456 (1999)
	The interacting Wolf-Rayet galaxy Mkn 8.
o	Table 2, Fig.1: <[EM99] NN> (Nos 1-20). Fig.4: <[EM99] A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: eMACS
eMACS	(extended Massive Cluster Survey)
*****	Avoid the usage of eMACS, prefer [EEB2013]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: eMACS
eMACS	(extended Massive Cluster Survey)
Write:	<<eMACS JHHMM.m+DDMM>>
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	The extended Massive Cluster Survey (eMACS) used X-ray detection coupled with optical confirmation to discover massive galaxy clusters. See also MCS, for the MAssive Cluster Survey (MACS). Only the first references are given here.
Ref:	=2013MNRAS.432...62E
by	EBELING H. , EDGE A.C., BURGETT W.S., CHAMBERS K.C., HODAPP K.W., HUBER M.E., KAISER N., PRICE P.A., TONRY J.L.
	Mon. Not. R. Astron. Soc., 432, 62-72 (2013)
	X-ray selected galaxy clusters in the Pan-STARRS Medium Deep Survey.
o	In Table A1, galaxy RX J1613.7+5542-g7 at z=0.3498 is [EEB2013] 1613.7+5542-g9 in SIMBAD; and galaxy RX J1613.7+5542-g7s is [EEB2013] 1613.7+5542-g9s.
o	Table 2: <eMACS JHHMM.m+DDMM> N=5 = <[EEB2013] eMACS JHHMM.m+DDMM> N=5. Table A1: <[EEB2013] eMACS JHHMM.m+DDMM-gNN>, <[EEB2013] eMACS JHHMM.m+DDMM-gNNs>, <[EEB2013] eMACS JHHMM.m+DDMM-xN>, <[EEB2013] RX JHHMM.m+DDMM-gNN>, <[EEB2013] RX JHHMM.m+DDMM-gNNs>, N=165.
Ref:	=2018ApJ...852L...7E
by	EBELING H. , STOCKMANN M., RICHARD J., ZABL J., BRAMMER G., TOFT S., MAN A.
	Astrophys. J., 852L, 7-7 (2018)
	Thirty-fold: extreme gravitational lensing of a quiescent galaxy at z = 1.6.
o	<eMACS JHHMM.m+DDMM> (No. J1341.9-2442) added. <[ESR2018] eMACSJ1341-QG-1> N=1. Fig. 1: <[ESR2018] eMACS J1341.9-2442 m1.N> (Nos m1.1-m1.3).
Ref:	=2020MNRAS.498.1121Z
by	ZALESKY L. , EBELING H.
	Mon. Not. R. Astron. Soc., 498, 1121-1139 (2020)
	AStroLens: automatic strong-lens modelling of X-ray selected galaxy clusters.
o	Tables 2+4: <eMACS JHHMM.m+DDMM> N=9+10 added.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EMB94]
[EMB94]	(Eisloffel+Mundt+Bohm, 1994)
Write:	<<[EMB94] HH 1 AJ>> <<[EMB94] HH 1 ANJ>>
N:	17
Object:	Knot (SIMBAD class: HerbigHaroObj = Herbig-Haro Object)
Stat:	is completely incorporated in Simbad
Note:	Knots in HH 1 Jet, format 'HH 1 AJ' or 'HH 1 ANJ', where the letter 'J' stands for Jet. See also [HSS98]
in source:	HH 1
Ref:	=1994AJ....108.1042E
by	EISLOEFFEL J. , MUNDT R., BOEHM K.-H.
	Astron. J., 108, 1042-1055 (1994)
	Structure and proper motions in Herbig-Haro objects 1 and 2.
o	The other knots in HH NN objects have a format 'HH NNA' or 'HH NNAN'
o	Fig.5, Table 2: <[EMB94] HH 1 AJ> (Nos AJ-GJ, XJ).
Ref:	=1996ApJ...468L.103R
by	RAY T.P. , MUNDT R., DYSON J.E., FALLE S.A.E.G., RAGA A.C.
	Astrophys. J., 468, 103-106 (1996)
	HST observations of jets from young stars.
o	The other knots in HH NN objects have a format 'HH NNA' or 'HH NNAN'
o	Fig.6: <[EMB94] HH 1 ANJ> (Nos G1J, G2J, HJ, I1J, I2J) added.
Ref:	=1998AJ....116..372H
by	HESTER J.J. , STAPELFELDT K.R., SCOWEN P.A.
	Astron. J., 116, 372-395 (1998)
	Hubble space telescope wide field planetary camera 2 observations of HH 1-2.
o	The other knots in HH NNN objects have a format 'HH NNNA' or 'HH NNNAN'. The 2 diffraction features 'D.S'' in Fig.6, without numbering, are not in SIMBAD.
o	Fig.3: <[EMB94] HH 1 ANJ> (Nos G3J, G4J, F1J, F2J) added. Figs 6, 7: <[HSS98] HH 1 Arch N> (Nos 1-3), <[HSS98] HH 1 Shoulder N> (Nos 1-2), <[HSS98] HH 1 Faint N> (Nos 1-2).
Ref:	=2005A&A...441..159N
by	NISINI B. , BACCIOTTI F., GIANNINI T., MASSI F., EISLOEFFEL J., PODIO L., RAY T.P.
	Astron. Astrophys., 441, 159-None (2005)
	A combined optical/infrared spectral diagnostic analysis of the HH1 jet.
o	Fig.1, Table 2: <[EMB94] HH 1 AJ> (Nos IJ to LJ) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EMD2009]
[EMD2009]	(Ellison+Murphy+Dessauges-Zavadsky, 2009) (Not yet in Simbad)
Write:	<<[EMD2009] QSO HHMM+DDdA abs N.NNN>> <<[EMD2009] QSO JHHMM+DDMM abs N.NNN>>
N:	56
Object:	Absorber
Note:	VLT UVES and Keck HIRES spectroscopy of DLAs and sub-DLAs.
Ref:	=2009MNRAS.392..998E
by	ELLISON S.L. , MURPHY M.T., DESSAUGES-ZAVADSKY M.
	Mon. Not. R. Astron. Soc., 392, 998-1007 (2009)
	The kinematic signature of damped Lyman α systems: using the D-index to screen for high column density HI absorbers.
o	Table 2: <[EMD2009] QSO HHMM+DDdA abs N.NNN>, <[EMD2009] QSO JHHMM+DDMM abs N.NNN> N=56.
=E=	Catalogue in electronic form as <J/MNRAS/392/998/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EMD2013]
[EMD2013]	(Ellis+McLure+Dunlop+, 2013)= (UDF12)
Write:	<<[EMD2013] UDF12-SSss-MSSs>>
N:	7
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=7 candidate z>8.5 galaxies from HST WFC3/IR images of the Hubble Ultra Deep Field (UDF), as part of the UDF2012 campaign. Format 'UDF12-SSss-MSSs': the complete 2000 coordinate format is 03 32 SS.ss (right ascension) and -27 4M SS.s (declination).
Ref:	=2013ApJ...763L...7E
by	ELLIS R.S. , McLURE R.J., DUNLOP J.S., ROBERTSON B.E., ONO Y., SCHENKER M.A., KOEKEMOER A., BOWLER R.A.A., OUCHI M., ROGERS A.B., CURTIS-LAKE E., SCHNEIDER E., CHARLOT S., STARK D.P., FURLANETTO S.R., CIRASUOLO M.
	Astrophys. J., 763L, 7 (2013)
	The abundance of star-forming galaxies in the redshift range 8.5-12: new results from the 2012 Hubble ultra deep field campaign.
o	Fig. 1, Table 1: <[EMD2013] UDF12-SSss-MSSs> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EME94]
[EME94]	(ELSTON+MCCARTHY+EISENHARDT+, 1994)
Write:	<<[EME94] COMP N>>
N:	3
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=3 COMPONENTS OF IRAS F10214+4724.
in source:	IRAS F10214+4724
Ref:	=1994AJ....107..910E
by	ELSTON R. , McCARTHY P.J., EISENHARDT P., DICKINSON M., SPINRAD H., JANNUZI B.T., MALONEY P.
	Astron. J., 107, 910-919 (1994)
	The Seyfert II nature of the IRAS source FSC 10214+4724.
o	Fig.4: Star A = [RBL91] A.
o	Table 2: <[EME94] Comp N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EMF2013]
[EMF2013]	(Elia+Molinari+Fukui+, 2013)= ([EMF2013a])
Write:	<<[EMF2013] GLLL.lllll+BB.bbbbb>>
N:	321+943
Object:	(Rad) + (FIR) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=321 clumps found in the NANTEN CO(1-0) Galactic Plane Survey data set. N=943 Hi-GAL sources (Herschel PACS and SPIRE observations).
Ref:	=2013ApJ...772...45E
by	ELIA D. , MOLINARI S., FUKUI Y., SCHISANO E., OLMI L., VENEZIANI M., HAYAKAWA T., PESTALOZZI M., SCHNEIDER N., BENEDETTINI M., DI GIORGIO A.M., IKHENAODE D., MIZUNO A., ONISHI T., PEZZUTO S., PIAZZO L., POLYCHRONI D., RYGL K.L.J., YAMAMOTO H., MARUCCIA Y.
	Astrophys. J., 772, 45 (2013)
	The first Hi-GAL observations of the outer galaxy: a look at star formation in the third galactic quadrant in the longitude range 216.°5 ≲ ℓ ≲ 225.°5.
o	Tables 2-3: <[EMF2013] GLLL.lllll+BB.bbbbb> N=321+943.
=E=	Catalogue in electronic form as J/ApJ/772/45
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EMF2013a]
[EMF2013a]	(Elia+Molinari+Fukui+, 2013)
*****	Avoid the usage of [EMF2013a], prefer [EMF2013]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EMF2013b]
[EMF2013b]	(Elyiv+Melnyk+Finet+, 2013)
Write:	<<[EMF2013b] JHHMMSS.s+DDMMSS>> <<[EMF2013b] JHHMMSS.s+DDMMSS A>>
N:	18+38
Object:	Poss. Grav. lens system + Poss. Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=18 gravitational lens candidates among some 5500 optical counterparts of the X-ray point-like sources in the medium-deep XMM-LSS survey.
Ref:	=2013MNRAS.434.3305E
by	ELYIV A. , MELNYK O., FINET F., POSPIESZALSKA-SURDEJ A., CHIAPPETTI L., PIERRE M., SADIBEKOVA T., SURDEJ J.
	Mon. Not. R. Astron. Soc., 434, 3305-3309 (2013)
	Search for gravitational lens candidates in the XMM-LSS/CFHTLS common field.
o	Table 1, Fig. 1: <[EMF2013b] JHHMMSS.s+DDMMSS> N=18, <[EMF2013b] JHHMMSS.s+DDMMSS A> N=38.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EMK2009]
[EMK2009]	(Ebeling+Ma+Kneib+, 2009)
Write:	<<[EMK2009] JHHMMSS.ss+DDMMSS.s>>
N:	62
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS1 and CFHT MOS spectroscopy of N=62 galaxies in the field of the galaxy cluster MCS J1206.2-0847.
in source:	MCS J1206.2-0847
Ref:	=2009MNRAS.395.1213E
by	EBELING H. , MA C.J., KNEIB J.-P., JULLO E., COURTNEY N.J.D., BARRETT E., EDGE A.C., LE BORGNE J.-F.
	Mon. Not. R. Astron. Soc., 395, 1213-1224 (2009)
	A spectacular giant arc in the massive cluster lens MACSJ1206.2-0847.
o	Table 1: <[EMK2009] JHHMMSS.ss+DDMMSS.s> N=62.
=E=	Catalogue in electronic form as <J/MNRAS/395/1213/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EML2004]
[EML2004]	(EIKENBERRY+MATTHEWS+LAVINE+, 2004)
Write:	<<[EML2004] STAR A>>
N:	4
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	OSIRIS CTIO observations. Photometry and spectroscopy of the star 'NAME LBV 1806-20' and three nearby stars.
Ref:	=2004ApJ...616..506E
by	EIKENBERRY S.S. , MATTHEWS K., LAVINE J.L., GARSKE M.A., HU D., JACKSON M.A., PATEL S.G., BARRY D.J., COLONNO M.R., HOUCK J.R., WILSON J.C., CORBEL S., SMITH J.D.
	Astrophys. J., 616, 506-518 (2004)
	Infrared observations of the candidate LBV 1806-20 and nearby cluster stars.
o	Fig.1, Table 1: <[EML2004] Star A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EMM2013]
[EMM2013]	(Eden+Moore+Morgan+, 2013)
Write:	<<[EMM2013] GRSMC GLLL.ll+BB.bb+VV.vv>>
N:	2
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	JCMT HARP 13CO(3-2) observations of N=2 molecular clouds.
Ref:	=2013MNRAS.431.1587E
by	EDEN D.J. , MOORE T.J.T., MORGAN L.K., THOMPSON M.A., URQUHART J.S.
	Mon. Not. R. Astron. Soc., 431, 1587-1595 (2013)
	Star formation in Galactic spiral arms and the interarm regions.
o	Table 3: <[EMM2013] GRSMC GLLL.ll+BB.bb+VV.vv> N=2.
o	Table 2: the BGPS source ID is the running catalog number (cf catalog J/ApJS/188/123/table1 in VizieR).
=E=	Catalogue in electronic form as J/MNRAS/431/1587
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EMNO
EMNO	(Extreme Mid-to-Near ir Object)
Write:	<<EMNO N>>
N:	9
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Extreme Mid-to-Near IR objects from the ELAISC15 survey.
Ref:	=2004A&A...427..795J
by	JOHANSSON P.H. , VAEISAENEN P., VACCARI M.
	Astron. Astrophys., 427, 795-801 (2004)
	A population of extreme mid-to-near-infrared sources: Obscured AGN and dusty starbursts.
o	Table 1: <EMNO N> (Nos 1-9).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EMR2006]
[EMR2006]	(Egami+Misselt+Rieke+, 2006)
Write:	<<[EMR2006] JHHMMSS.s+DDMMSS>>
N:	11
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC and MIPS observations of the Brightest Cluster Galaxy (BCG) in 11 clusters.
Ref:	=2006ApJ...647..922E
by	EGAMI E. , MISSELT K.A., RIEKE G.H., WISE M.W., NEUGEBAUER G., KNEIB J.-P., LE FLOC'H E., SMITH G.P., BLAYLOCK M., DOLE H., FRAYER D.T., HUANG J.-S., KRAUSE O., PAPOVICH C., PEREZ-GONZALEZ P.G., RIGBY J.R.
	Astrophys. J., 647, 922-933 (2006)
	Spitzer observations of the brightest galaxies in X-ray-luminous clusters.
o	Table 1, col(2,4): <[EMR2006] JHHMMSS.s+DDMMSS> N=11.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EMS2007]
[EMS2007]	(Elia+Massi+Strapella+, 2007)= ([EMS2007a])
Write:	<<[EMS2007] VMR-DNN>>
N:	49
Object:	CO Clump (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	CO line maps obtained with the SEST of the VMR D region.
in source:	VMR D
Ref:	=2007ApJ...655..316E
by	ELIA D. , MASSI F., STRAFELLA F., DE LUCA M., GIANNINI T., LORENZETTI D., NISINI B., CAMPEGGIO L., MAIOLO B.M.T.
	Astrophys. J., 655, 316-331 (2007)
	Mapping molecular emission in Vela molecular ridge cloud D.
o	Fig.9: objects M55 23 not identified.
o	Table 3: <[EMS2007] VMR-DNN> (Nos D1-D49).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EMS2007a]
[EMS2007a]	(Elia+Massi+Strapella+, 2007)
*****	Avoid the usage of [EMS2007a], prefer [EMS2007]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EMS2007b]
[EMS2007b]	(Eastman+Martini+Sivakoff+, 2007)
Write:	<<[EMS2007b] MS2053-XN>>
N:	5
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra X-ray sources at the redshift of ClG 2053-0449.
in source:	1E 2053.7-0449 = ClG 2053-0449
Ref:	=2007ApJ...664L...9E
by	EASTMAN J. , MARTINI P., SIVAKOFF G., KELSON D.D., MULCHAEY J.S., TRAN K.-V.
	Astrophys. J., 664L, 9-12 (2007)
	First measurement of a rapid increase in the AGN fraction in high-redshift clusters of galaxies.
o	Text: The cluster 0848.6+4453 (ClG 0848+4453 in SIMBAD) has a z = 1.273, and the cluster 0848.8+4456 (ClG J0848+4456 in SIMBAD) a z = 0.57. Table 2: CXOSEXSI sources seem to be in ClG 0848+4456. (See 1999AJ....118...76R, table 1)
o	Table 1: <[EMS2007b] MS2053-XN> (Nos X1 to X5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EMSS
EMSS	(Extended Medium Sensitivity Survey)
====>	Equivalent to: 1E
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EMU
EMU	(Evolutionary Map of the Universe)
Write:	<<EMU NA JHHMMSS.s+DDMMSS>>
N:	about 70 million (SIMBAD class: cmRad = Centimetric Radio Source)
Note:	EMU is a new radio survey with the nearly completed ASKAP telescope, which is expected to produce a catalogue of about 70 million radio components (i.e. a blob of radio emission), which will then be grouped into about 63 million radio sources (i.e. a physical object, typically a host galaxy). Our wiki is http://askap.pbworks.com
Notes:	The N in the designation is the catalog version number. The A following may either be blank (meaning a component) or the letter S meaning a source. We may later add other letters such as D for diffuse source. I'd welcome comments and suggestions on this.
Ref:	=2011PASA...28..215N
Auth.:	Ray Norris CSIRO/Western Sydney Uni
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [EMU2018]
[EMU2018]	(Eden+Moore+Urquhart+, 2018)
Write:	<<[EMU2018] W49 NNN>> <<[EMU2018] Hi-GAL NNNNNN>>
N:	173+57+434
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	JCMT SCUBA-2 850µm observations of N=173 compact sources in W49A. N=57+434 compact sources in W49A and W51, using Hi-GAL data.
in source:	W 49:W 49A = W 49A
in source:	W 51
Ref:	=2018MNRAS.477.3369E
by	EDEN D.J. , MOORE T.J.T., URQUHART J.S., ELIA D., PLUME R., KONIG C., BALDESCHI A., SCHISANO E., RIGBY A.J., MORGAN L.K., THOMPSON M.A.
	Mon. Not. R. Astron. Soc., 477, 3369-3382 (2018)
	Extreme star formation in the Milky Way: luminosity distributions of young stellar objects in W49A and W51.
o	Table 2: <[EMU2018] W49 NNN> N=171 among (Nos 001-173), Nos 040, 093 missing. Tables B2-B3: <[EMU2018] Hi-GAL NNNNNN> N=57+434 among (Nos 180502-182333, 196057-201478).
=E=	Catalogue in electronic form as <J/MNRAS/477/3369/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EMV2004]
[EMV2004]	(Eckart+Moultaka+Viehmann+, 2004)
Write:	<<[EMV2004] ggg>>
N:	8
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	VLT observations. N=8 new IR sources in the GCIRS 13 complex in the Galactic Center.
in source:	NAME Gal Center
Ref:	=2004ApJ...602..760E
by	ECKART A. , MOULTAKA J., VIEHMANN T., STRAUBMEIER C., MOUAWAD N.
	Astrophys. J., 602, 760-769 (2004)
	Young stars at the center of the Milky way.
o	Table 2: <[EMV2004] aaa> N=8. Table 2: <GCIRS NNWNa> (No. 13E3c>, <GCIRS NNWNW> (No. 13E3N>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EMY2013]
[EMY2013]	(Eckart+Muzic+Yazici+, 2013) (Not yet in Simbad)
Write:	<<[EMY2013] NN>>
N:	33
Object:	(NIR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	ESO VLT SINFONI observations of the Galactic Center.
in source:	NAME Galactic Center
Ref:	=2013A&A...551A..18E
by	ECKART A. , MUZIC K., YAZICI S., SABHA N., SHAHZAMANIAN B., WITZEL G., MOSER L., GARCIA-MARIN M., VALENCIA-S. M., JALALI B., BREMER M., STRAUBMEIER C., RAUCH C., BUCHHOLZ R., KUNNERIATH D., MOULTAKA J.
	Astron. Astrophys., 551A, 18-18 (2013)
	Near-infrared proper motions and spectroscopy of infrared excess sources at the Galactic center.
o	Fig. 2, Table 3: <[EMY2013] NN> (Nos 1-33).
o	S54, 56, 79 and 90 are not in Simbad (no coordinates).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EN1
EN1	(ELAIS N1)
*****	Avoid the usage of EN1, prefer [RLP2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ENACS
ENACS	(ESO Nearby Abell Cluster Survey)
Write:	<<ENACS ACO NNNN NNN>>
N:	5634
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=5634 galaxies in 107 ACO clusters
Ref:	=1998A&AS..129..399K
by	KATGERT P. , MAZURE A., DEN HARTOG R., ADAMI C., BIVIANO A., PEREA J.
	Astron. Astrophys., Suppl. Ser., 129, 399-412 (1998)
	The ESO Nearby Abell Cluster Survey. V. The catalogue: Contents and instructions for use.
o	Catalogue: <ENACS ACO NNNN NNN> N=5634
=E=	Catalogue in electronic form as J/A+AS/129/399
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ENF2003]
[ENF2003]	(English+Norris+Freeman+, 2003)
Write:	<<[ENF2003] AN>>
N:	9
Object:	HI (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	N=9 HI spatial fragments around NGC 3256. See also paper I: [EF2003].
in source:	NGC 3256
Ref:	=2003AJ....125.1134E
by	ENGLISH J. , NORRIS R.P., FREEMAN K.C., BOOTH R.S.
	Astron. J., 125, 1134-1149 (2003)
	NGC 3256: kinematic anatomy of a merger.
o	Fig.5, Table 2: <[ENF2003] AN> (Nos A1-A9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ENM96]
[ENM96]	(Ellingsen+Norris+McCulloch, 1996)
Write:	<<[ENM96] JHHMMSS.sss+DDMMSS.ss>>
N:	5
Object:	CH3OH Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	N=5 CH3OH masers in 5 HII regions.
Ref:	=1996MNRAS.279..101E
by	ELLINGSEN S.P. , NORRIS R.P., McCULLOCH P.M.
	Mon. Not. R. Astron. Soc., 279, 101-107 (1996)
	Continuum emission associated with 6.7-GHz methanol masers.
o	Table 1: 2 first objects are PMN, 1744-312 not identified.
o	Table 2: <[ENM96] JHHMMSS.sss+DDMMSS.ss> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EO
EO	(Extended Object)
Write:	<<EO NGC NNNN NNN>> <<EO NGC NNNN/N NNN>> <<EO APG 141 NNN>>
N:	1444
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	'Extended Objects', dwarf galaxy candidates, near 14 galaxies or group of galaxies
Ref:	=1998A&AS..129..455D
by	DEEG H.J. , MUNOZ-TUNON C., TENORIO-TAGLE G., TELLES E., VILCHEZ J.M., RODRIGUEZ-ESPINOSA J.M., DUC P.A., MIRABEL I.F.
	Astron. Astrophys., Suppl. Ser., 129, 455-462 (1998)
	A catalogue of dwarf galaxy candidates around interacting galaxies.
o	<EO NGC NNNN NNN>, <EO NGC NNNN/N NNN>, <EO APG 141 NNN>, N=1444.
=E=	Catalogue in electronic form as J/A+AS/129/455
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EOK2015]
[EOK2015]	(Evans+Osborne+Kennea+, 2015)
Write:	<<[EOK2015] NN NN>>
N:	109
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Swift XRT detection of N=109 X-ray sources of 20 IceCube neutrino-doublet triggers.
Ref:	=2015MNRAS.448.2210E
by	EVANS P.A. , OSBORNE J.P., KENNEA J.A., SMITH M., PALMER D.M., GEHRELS N., GELBORD J.M., HOMEIER A., VOGE M., STROTJOHANN N.L., COWEN D.F., BOSER S., KOWALSKI M., STASIK A.
	Mon. Not. R. Astron. Soc., 448, 2210-2223 (2015)
	Swift follow-up of IceCube triggers, and implications for the Advanced-LIGO era.
o	Table 2: <[EOK2015] NN NN> N=109.
=E=	Catalogue in electronic form as J/MNRAS/448/2210
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EON
EON	(Edge-ON disk galaxies)
Write:	<<EON DDD.ddd+DD.ddd>> <<EON EON_DDD.ddd_+DD.ddd>> (not recognised by Simbad, but found in literature)
N:	5750
Object:	G (SIMBAD class: Galaxy)
Note:	Catalog of N=5750 edge-on disk galaxies. Use of archival SDSS images.
Ref:	=2014ApJ...787...24B
by	BIZYAEV D.V. , KAUTSCH S.J., MOSENKOV A.V., RESHETNIKOV V.P., SOTNIKOVA N.Ya., YABLOKOVA N.V., HILLYER R.W.
	Astrophys. J., 787, 24 (2014)
	The catalog of edge-on disk galaxies from SDSS. I. The catalog and the structural parameters of stellar disks.
o	Table 4: <EON DDD.ddd+DD.ddd> N=5750.
=E=	Catalogue in electronic form as J/ApJ/787/24
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EOri
EOri	(Eps Ori cluster)
Write:	<<EOri N-NNNN>>
N:	3+6
Object:	* in Cl* (SIMBAD class: Star)
Note:	Search for stars in the eps Ori Cluster form an unpublished catalog of Bejar. See also Annizam, Mantaqah.
in source:	NAME eps Ori Cluster
Ref:	=2008A&A...485..931C
by	CABALLERO J.A. , SOLANO E.
	Astron. Astrophys., 485, 931-949 (2008)
	Young stars and brown dwarfs surrounding Alnilam (ε Orionis) and Mintaka (δ Orionis).
o	Notes to table A.6 p.943 TYC 4767-2257-1 is a probable misprint for TYC 4766-757-1
o	Tables a9, a11: <EOri N-NNNN> N=9. Tables a9, a16: <Annizam NNNNNN> N=181. Tables a10, a17: <Mantaqah NNNNNNN> N=103.
=E=	Catalogue in electronic form as <J/A+A/485/931/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EP2013]
[EP2013]	(Ehlerova+Palous, 2013)= (GSH)
Write:	<<[EP2013] GLLL.l+BB.b+VVV.v>>
N:	333
Object:	HI Shell (SIMBAD class: HIshell = Interstellar Shell)
Note:	N=333 HI shells identified in the all-sky Leiden/Argentina/Bonn HI survey. The format is based on the galactic coordinates of the centre of the structure and the radial velocity.
Ref:	=2013A&A...550A..23E
by	EHLEROVA S. , PALOUS J.
	Astron. Astrophys., 550A, 23-23 (2013)
	HI shells in the Leiden/Argentina/Bonn HI survey.
o	Tables A.1-A.2: <[EP2013] GLLL.l+BB.b+VVV.v> N=333.
=E=	Catalogue in electronic form as J/A+A/550/A23
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EP97]
[EP97]	(Eskridge+Pogge, 1997)= ([EP97a]) (Not yet in Simbad)
Write:	<<[EP97] RNa>>
N:	11
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Map in Fig.1
in source:	NGC 2685
Ref:	=1997ApJ...486..259E
by	ESKRIDGE P.B. , POGGE R.W.
	Astrophys. J., 486, 259-267 (1997)
	H II region abundances in the polar ring of NGC 2685.
o	Table 4: <[EP97] RNa> (Nos R1-R7, R8a-R8c, R9)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EP97a]
[EP97a]	(Eskridge+Pogge, 1997) (Not yet in Simbad)
*****	Avoid the usage of [EP97a], prefer [EP97]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EP97b]
[EP97b]	(El-Ad+Piran, 1997)
Write:	<<[EP97b] NN>>
N:	18
Object:	Void (SIMBAD class: Void = Underdense Region of the Universe)
Stat:	is completely incorporated in Simbad
Note:	N=18 Voids in the SSRS2 survey. See also [DPS88] voids in the SSRS survey
Ref:	=1997ApJ...491..421E
by	EL-AD H. , PIRAN T.
	Astrophys. J., 491, 421-435 (1997)
	Voids in the large-scale structure.
o	Table 1: <[EP97b] NN> (Nos 1-18)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EPB95]
[EPB95]	(Ehle+Pietsch+Beck, 1995)
Write:	<<[EPB95] NN>>
N:	16
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations. Table 2: N=16 sources in M 51, sources 11 and 13 are in NGC 5195
in source:	M 51 = NGC 5194
Ref:	=1995A&A...295..289E
by	EHLE M. , PIETSCH W., BECK R.
	Astron. Astrophys., 295, 289-301 (1995)
	ROSAT high-resolution X-ray observations of the galaxies M51 and NGC5195.
o	Table 2: <[EPB95] NN> N=19
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EPB98]
[EPB98]	(Ehle+Pietsch+Beck+, 1998)
Write:	<<[EPB98] NN>>
N:	47
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations. See also HRI sources: [IVE99].
in source:	M 83 = NGC 5236
Ref:	=1998A&A...329...39E
by	EHLE M. , PIETSCH W., BECK R., KLEIN U.
	Astron. Astrophys., 329, 39-54 (1998)
	ROSAT PSPC X-ray observations of the nearby spiral galaxy M 83.
o	Table 4: <[EPB98] NN> (Nos 1-47)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EPD97]
[EPD97]	(El-Ad+Piran+Da Costa, 1997) (Not yet in Simbad)
Write:	<<[EPD97] NN>>
N:	15
Object:	Void (SIMBAD class: Void = Underdense Region of the Universe)
Ref:	=1997MNRAS.287..790E
by	EL-AD H. , PIRAN T., DA COSTA L.N.
	Mon. Not. R. Astron. Soc., 287, 790-798 (1997)
	A catalogue of the voids in the IRAS 1.2-Jy survey.
o	Table 1: <[EPD97] NN> (Nos 1-15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EPF2014]
[EPF2014]	(Erfanianfar+Popesso+Finoguenov+, 2014)
Write:	<<[EPF2014] NN>>
N:	27
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	N=27 X-ray selected groups of galaxies catalogue. Use of Chandra and XMM-Newton data.
in source:	NAME COSMOS field
in source:	NAME ECDF
in source:	NAME CDFN
Ref:	=2014MNRAS.445.2725E
by	ERFANIANFAR G. , POPESSO P., FINOGUENOV A., WUYTS S., WILMAN D., BIVIANO A., ZIPARO F., SALVATO M., NANDRA K., LUTZ D., ELBAZ D., DICKINSON M., TANAKA M., MIRKAZEMI M., BALOGH M.L., ALTIERI M.B., AUSSEL H., BAUER F., BERTA S., BIELBY R.M., BRANDT N., CAPPELLUTI N., CIMATTI A., COOPER M., FADDA D., ILBERT O., LE FLOCH E., MAGNELLI B., MULCHAEY J.S., NORDON R., NEWMAN J.A., POGLITSCH A., POZZI F.
	Mon. Not. R. Astron. Soc., 445, 2725-2745 (2014)
	The evolution of star formation activity in galaxy groups.
o	Table A.1: <[EPF2014] NN> N=27 among (Nos 2-34).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EPH2001]
[EPH2001]	(Ehlerova+Palous+Huchtmeier, 2001)
Write:	<<[EPH2001] LL.l+B.b+VV>>
N:	4
Object:	HI Shell (SIMBAD class: HIshell = Interstellar Shell)
Stat:	is completely incorporated in Simbad
Note:	N=4 neighbours of GSH 061+99+51.
Ref:	=2001A&A...374..682E
by	EHLEROVA S. , PALOUS J., HUCHTMEIER W.K.
	Astron. Astrophys., 374, 682-690 (2001)
	The HI supershell GS061+00+51 and its neighbours.
o	<[EPH2001] LL.l+B.b+VV> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EPIC
EPIC	(Ecliptic Plane Input Catalog)
Write:	<<EPIC NNNNNNNNN>>
N:	about 28 millions
Object:	* (SIMBAD class: Star)
Note:	The Ecliptic Plane Input Catalog (EPIC) for Kepler's K2 mission (K2: Extending Kepler?s Power to the Ecliptic, see http://keplerscience.arc.nasa.gov/K2/). This catalog plays the same role for K2 that the Kepler Input Catalog (KIC) played for Kepler target selection. IDs begin at 201 million and go up to more than 220 million. The EPIC catalog is hosted at MAST (http://archive.stsci.edu/k2/epic/search.php).
=E=	Catalogue in electronic form as <IV/34/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EPIC
EPIC	(Ecliptic Plane Input Catalog)
Write:	<<EPIC NNNNNNNNN.NN>> <<EPIC NNNNNNNNN a>>
Object:	Poss. Planet (SIMBAD class: Planet_Candidate = Extra-solar Planet Candidate)
Note:	EPIC numbering for potential planets oribiting EPIC stars, observed during the extended Kepler mission K2. Both notations are used in the NASA Exoplanet Archive (https://exoplanetarchive.ipac.caltech.edu/). Following the Kepler prime mission convention, K2 candidates are identified by appending a two-digit identifier sequence number after the host star's EPIC identifier, separated by a period: e.g., EPIC 205071984.02 (=K2-32 d).
Origin	of the Acronym: L (2015ApJ...809...25M)
Details on Acronym: EPIC
EPIC	(European Photon Imaging Camera)
*****	Avoid the usage of EPIC, prefer [SD2005]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EPM2011]
[EPM2011]	(Ellison+Prochaska+Mendel, 2011) (Not yet in Simbad)
Write:	<<[EPM2011] QSO JHHMMSS.ss+DDMMSS.s abs N.NNNNN>>
N:	85
Object:	DLA
Note:	N=85 proximate absorbers in the Sloan Digital Sky Survey.
Ref:	=2011MNRAS.412..448E
by	ELLISON S.L. , PROCHASKA J.X., MENDEL J.T.
	Mon. Not. R. Astron. Soc., 412, 448-468 (2011)
	Metallicities and dust content of proximate damped Lyman α systems in the Sloan digital sky survey.
o	Table 1: <[EPM2011] QSO JHHMMSS.ss+DDMMSS.s abs N.NNNNN> N=85.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EPN
EPN	(Extragalactic Planetary Nebulae) >>>>>> New acronym being registered
Object:	PN
Auth.:	ACKER A.+
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [EPR2003]
[EPR2003]	(Engargiola+Plambeck+Rosolowsky+, 2003)= (EPRB)
Write:	<<[EPR2003] NNN>>
N:	148
Object:	Giant MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	BIMA observations. Catalog of 148 giant molecular clouds in M 33.
in source:	M 33 = NGC 598
Ref:	=2003ApJS..149..343E
by	ENGARGIOLA G. , PLAMBECK R.L., ROSOLOWSKY E., BLITZ L.
	Astrophys. J., Suppl. Ser., 149, 343-363 (2003)
	Giant molecular clouds in M33. I. BIMA all-disk survey.
o	Table 1: <[EPR2003] NNN> (Nos 1-148).
=E=	Catalogue in electronic form as J/ApJS/149/343
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EPRB
EPRB	(Engargiola+Plambeck+Rosolowsky+Blitz)
*****	Avoid the usage of EPRB, prefer [EPR2003]
Origin	of the Acronym: L (2003ApJ...599..258R)
Details on Acronym: eps Cha
eps Cha	(eps Cha Group)
*****	Avoid the usage of eps Cha, prefer [FLG2003]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EPS2001]
[EPS2001]	(Ellison+Pettini+Steidel+, 2001)
Write:	<<[EPS2001] QSO J0203+1134 abs N.NNNNN>> <<[EPS2001] 0201+1120 GN>> <<[EPS2001] 0201+1120 aAN>> <<[EPS2001] 0201+1120 aAANN>> <<[EPS2001] 0201+1120 aNN>>
N:	1+3+4
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck LRIS observations. Search for the system responsible for the z(abs) DLA system in the line of sight of QSO 0201+1120 = QSO J0203+1134. The system includes numerous galaxies.
Ref:	=2001ApJ...549..770E
by	ELLISON S.L. , PETTINI M., STEIDEL C.C., SHAPLEY A.E.
	Astrophys. J., 549, 770-779 (2001)
	An imaging and spectroscopic study of the z_{abs}=3.38639 damped Lyα system in Q0201+1120: clues to star formation at high redshift.
o	Text: <[EPS2001] QSO J0203+1134 abs 3.38639> N=1. Figs 2, 3, Table 2: <[EPS2001] 0201+1120 GN> (Nos G1-G3), <[EPS2001] 0201+1120 aAANN> (Nos oM6, oMD26), <[EPS2001] 0201+1120 aNN> (Nos m32, c10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EPS2012]
[EPS2012]	(EDWARDS+PAGNOTTA+SCHAEFER, 2012)
Write:	<<[EPS2012] NNN>> <<[EPS2012] RG>> <<[EPS2012] SG>>
N:	127+1+1
Object:	* + Red Giant + Supergiant (SIMBAD class: Star)
Note:	HST ACS observations of SNR B0519-69.0. See also [SP2012] and [PS2015].
in source:	SNR B0519-69.0
Ref:	=2012ApJ...747L..19E
by	EDWARDS Z.I. , PAGNOTTA A., SCHAEFER B.E.
	Astrophys. J., 747L, 19 (2012)
	The progenitor of the type Ia supernova that created SNR 0519-69.0 in the Large Magellanic Cloud.
o	Table 2: <[EPS2012] NNN> (Nos 1-127), <[EPS2012] RG> N=1, <[EPS2012] SG> N=1.
=E=	Catalogue in electronic form as <J/ApJ/747/L19/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EPV2015]
[EPV2015]	(Eigenthaler+Ploeckinger+Verdugo+, 2015)
Write:	<<[EPV2015] HCG NN a>>
N:	15
Object:	Tidal dwarf galaxy candidate (SIMBAD class: Galaxy_Candidate = Galaxy Candidate)
Stat:	is completely incorporated in Simbad
Note:	SOAR 4.1m telescope narrowband Halpha observations of N=15 tidal dwarf galaxy (TDG) candidates in three group of galaxies, HCG 26, HCG 91 and HCG 96.
in source:	HCG 26
in source:	HCG 91
in source:	HCG 96
Ref:	=2015MNRAS.451.2793E
by	EIGENTHALER P. , PLOECKINGER S., VERDUGO M., ZIEGLER B.
	Mon. Not. R. Astron. Soc., 451, 2793-2813 (2015)
	Star formation properties of Hickson Compact Groups based on deep Hα imaging.
o	Table 7: <[EPV2015] HCG NN a> N=15.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EPW2016]
[EPW2016]	(Evans+Pillitteri+Wolk+, 2016)
Write:	<<[EPW2016] l Car 1>> <<[EPW2016] A CCC N>> <<[EPW2016] VNNN CCC N>>
N:	30
Object:	* (SIMBAD class: Star)
Note:	HST WFC3 and XMM-Newton observations of N=30 candidate companions to 14 Galactic Cepheids.
Ref:	=2016AJ....151..108E
by	EVANS N.R. , PILLITTERI I., WOLK S., KAROVSKA M., TINGLE E., GUINAN E., ENGLE S., BOND H.E., SCHAEFER G.H., MASON B.D.
	Astron. J., 151, 108 (2016)
	Resolved companions of Cepheids: testing the candidates with X-ray observations.
o	Table 2: <[EPW2016] a CCC N>, <[EPW2016] A CCC N>, <[EPW2016] VNNN CCC N>, N=30.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EQ
EQ	(Equatorial coord.)
Write:	<<EQ HHMM+DD>> <<EQ HHMM+DDd>> <<EQ HHMM+DDdA>> <<EQ HHMM.m+DDd>> <<EQ HHMM.m+DDMM>> <<EQ HHMMSS+DDd>> <<EQ HHMM+DDMM>> <<EQ HHMM+DDMMSS>> <<EQ HHMM.m+DDMM>> <<EQ HHMMSS+DDMM>> <<EQ HHMMSS+DDMMm>> <<EQ HHMMSS+DDMMSS>> <<EQ HHMMSS+DDMMSS.s>> <<EQ HHMMSS.s+DDMMSS.s>> <<EQ JHHMM+DD>> <<EQ JHHMM+DDd>> <<EQ JHHMM.m+DDd>> <<EQ JHHMMSS+DDd>> <<EQ JHHMM+DDMM>> <<EQ JHHMM.m+DDMM>> <<EQ JHHMMSS+DDMM>> <<EQ JHHMMSS+DDMMSS>> <<EQ JHHMMSS+DDMMSS.s>> <<EQ JHHMMSS.s+DDMMSS.s>>
Object:	Unknown (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Systematic designation, in SIMBAD only. Acronym to avoid in the literature.
Details on Acronym: [EQL98]
[EQL98]	(Esamdin+Qiu+Li+, 1998)= (BAO)
Write:	<<[EQL98] N>>
N:	4
Object:	Catacl. V* (SIMBAD class: CataclyV* = Cataclysmic Binary)
Stat:	is completely incorporated in Simbad
Note:	Finding charts.
Ref:	=1998AcApS..18..214E
by	ESAMDIN A. , QIU Y.-L., LI W.-D., QIAO Q.-Y., WEI J.-Y., CAO L., HU J.-Y.
	Acta Astrophys. Sinica, 18, 214-216 (1998)
	The discovery of four cataclysmic variable stars in 1997 at Beijing Observatory.
o	Table 1: <[EQL98] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EQR2017]
[EQR2017]	(Ebeling+Qi+Richard, 2017)
Write:	<<[EQR2017] MACSJ0553-W>> <<[EQR2017] MACSJ0553-JFG1>> <<[EQR2017] MACSJ0553-W-BCG>> <<[EQR2017] NN.N>>
N:	2+1+2+10+30
Object:	Subcluster of G + G + Brightest Cluster Galaxy + Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST WFPC2 and ACS imaging, Keck-I and Keck-II LRIS and DEIMOS spectroscopy of the field of the galaxy cluster MCS J0553.4-3342: N=2 subclusters of galaxies, N=1 jellyfish galaxy, N=2 brightest cluster galaxies, and N=30 gravitationally lensed images in N=10 multiple-image systems. See also MACSg for other galaxies in the field of MCS J0553.4-3342.
in source:	MCS J0553.4-3342
Ref:	=2017MNRAS.471.3305E
by	EBELING H. , QI J., RICHARD J.
	Mon. Not. R. Astron. Soc., 471, 3305-3322 (2017)
	Fully stripped? The dynamics of dark and luminous matter in the massive cluster collision MACSJ0553.4-3342.
o	<[EQR2017] MACSJ0553-W> (Nos E, W). Paragr. 6.1.2, Table A1: <[EQR2017] MACSJ0553-JFG1> N=1. Table A1: <[EQR2017] MACSJ0553-W-BCG> (Nos E-BCG, W-BCG). Fig. 6, Table 3: <[EQR2017] NN.N> (Nos 1-10, 1.1-1.3 to 10.1-10.3). Table A.1: <MACSg JHHMMSS.s+DDMMSS> N=90.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EQS
EQS	(Edinburgh Quasar Survey)
Write:	<<EQS BHHMM+DDMM>>
N:	87
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	Sample of 87 QSOs selected from the EQS.
Ref:	=1999ApJ...511..612G
by	GOLDSCHMIDT P. , KUKULA M.J., MILLER L., DUNLOP J.S.
	Astrophys. J., 511, 612-624 (1999)
	A comparison of the optical properties of radio-loud and radio-quiet quasars.
o	Table 1: <EQS BHHMM+DDMM> N=87.
=E=	Catalogue in electronic form as J/ApJ/511/612
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ER
ER	(Extremely Red object)
*****	Avoid the usage of ER, prefer [FSL2005]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ER96]
[ER96]	(Eales+Rawlings, 1996)
Write:	<<[ER96] 6C 0930+38 a>> <<[ER96] 6C 1031+34 a>> <<[ER96] MG 2141+192 a>>
N:	3+2+2
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Figs 2: Faint objects in the field of 6C 0930+38 = 6C 0930+3855: N=3, (Nos a-c). 6C 1031+34 = 6C 1031+3404: N=2, (Nos a-b). MG 2141+192 = MITG J2144+929: N=2, (Nos a-b)
Ref:	=1996ApJ...460...68E
by	EALES S.A. , RAWLINGS S.
	Astrophys. J., 460, 68-93 (1996)
	A panoramic view of radio galaxy evolution from a redshift of 0 to a redshift of 4.3.
o	MG 2141+192 = MITG J2144+1929, B3 0731+43 = B3 0731+438, MG 1744+18 = MITG J1747+1821, 6C 0930+38 = 6C 0930+3855, 6C 1031+34 = 6C 1031+3404
o	Fig.2i: <[ER96] 6C 0930+38 a> (Nos a-c). Fig.2j: <[ER96] 6C 1031+34 a> (Nos a-b). Fig.2n: <[ER96] MG 2141+192 a> (Nos a-b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 1eRASS
1eRASS	(eROSITA source detected in the first all sky survey)
Write:	<<1eRASS JHHMMSS.s+DDMMSS>>
N:	about 1400000
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	The eROSITA telescope array aboard the Spektrum Roentgen Gamma (SRG) satellite began surveying the sky in December 2019, with the aim of producing all-sky X-ray source lists and sky maps of unprecedented depth. The Designation covers all sources detected in the data acquired in the first six months of survey operations (eRASS1; completed June 2020) over the half-sky whose proprietary data rights lie with the German eROSITA Consortium.
Ref:	=2024A&A...682A..34M
by	MERLONI A. , LAMER G., LIU T., RAMOS-CEJA M.E., BRUNNER H., BULBUL E., DENNERL K., DOROSHENKO V., FREYBERG M.J., FRIEDRICH S., GATUZZ E., GEORGAKAKIS A., HABERL F., IGO Z., KREYKENBOHM I., LIU A., MAITRA C., MALYALI A., MAYER M.G.F., NANDRA K., PREDEHL P., ROBRADE J., SALVATO M., SANDERS J.S., STEWART I., TUBIN-ARENAS D., WEBER P., WILMS J., ARCODIA R., ARTIS E., ASCHERSLEBEN J., AVAKYAN A., AYDAR C., BAHAR Y.E., BALZER F., BECKER W., BERGER K., BOLLER T., BORNEMANN W., BRUGGEN M., BRUSA M., BUCHNER J., BURWITZ V., CAMILLONI F., CLERC N., COMPARAT J., COUTINHO D., CZESLA S., DANNHAUER S.M., DAUNER L., DAUSER T., DIETL J., DOLAG K., DWELLY T., EGG K., EHL E., FREUND S., FRIEDRICH P., GAIDA R., GARREL C., GHIRARDINI V., GOKUS A., GRUNWALD G., GRANDIS S., GROTOVA I., GRUEN D., GUEGUEN A., HAMMERICH S., HAMAUS N., HASINGER G., HAUBNER K., HOMAN D., IDER CHITHAM J., JOSEPH W.M., JOYCE A., KONIG O., KALTENBRUNNER D.M., KHOKHRIAKOVA A., KINK W., KIRSCH C., KLUGE M., KNIES J., KRIPPENDORF S., KRUMPE M., KURPAS J., LI P., LIU Z., LOCATELLI N., LORENZ M., MULLER S., MAGAUDDA E., MANNES C., McCALL H., MEIDINGER N., MICHAILIDIS M., MIGKAS K., MUNOZ-GIRALDO D., MUSIIMENTA B., NGUYEN-DANG N.T., NI Q., OLECHOWSKA A., OTA N., PACAUD F., PASINI T., PERINATI E., PIRES A.M., POMMRANZ C., PONTI G., POPPENHAEGER K., PUHLHOFER G., RAU A., REH M., REIPRICH T.H., ROSTER W., SAEEDI S., SANTANGELO A., SASAKI M., SCHMITT J., SCHNEIDER P.C., SCHRABBACK T., SCHUSTER N., SCHWOPE A., SEPPI R., SERIM M.M., SHREERAM S., SOKOLOVA-LAPA E., STARCK H., STELZER B., STIERHOF J., SULEIMANOV V., TENZER C., TRAULSEN I., TRUMPER J., TSUGE K., URRUTIA T., VERONICA A., WADDELL S.G.H., WILLER R., WOLF J., YEUNG M.C.H., ZAINAB A., ZANGRANDI F., ZHANG X., ZHANG Y., ZHENG X.
	Astron. Astrophys., 682A, 34 (2024)
	The SRG/eROSITA all-sky survey First X-ray catalogues and data release of the western Galactic hemisphere.
o	<1eRASS JHHMMSS.s+DDMMSS> N=930203+347274+5466. Max-Planck-Institute for Extraterrestrial Physic
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: eRASSt
eRASSt	(eRASSt)
Write:	<<eRASSt JHHMMSS+DDMMSS>> <<eRASSt JHHMMSS.s+DDMMSS>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	SRG eROSITA observations of X-ray sources in the eROSITA all-sky surveys (eRASS). See also eRASSU. Only the first references are listed here.
Ref:	=2020ATel13712....1M
by	MALYALI A. , RAU A., ARCODIA R., BOLLER T., CARPANO S., HABERL F., MERLONI A., NANDRA K., BUCHNER J., LIU T., SALVATO M., WILMS J., KOENIG O., KRUMPE M., LAMER G.
	ATel, 3712, 1 (2020)
	eRASSt J082337+042303: A bright, ultra-soft, high-amplitude transient in the direction of 2MASX J08233674+042300.
o	<eRASSt JHHMMSS+DDMMSS> N=1.
Ref:	=2020ATel13844....1R
by	RAU A. , MAITRA C., DUCCI L., SCHMITT J., WILMS J., KREYKENBOHM I., WEBER P., SALVATO M., LAMER G., SCHWOPE A.
	ATel, 3844, 1 (2020)
	eRASSt J100130.9-614021: A new bright X-ray source discovered by SRG/eROSITA.
o	<eRASSt JHHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: eRASSU
eRASSU	(eRASSU)
Write:	<<eRASSU JHHMMSS.s+DDMMSS>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	SRG eROSITA observations of X-ray sources in the eROSITA all-sky surveys (eRASS). See also eRASSt. Only the first references are listed here.
Ref:	=2020ATel13609....1H
by	HABERL F. , MAITRA C., CARPANO S., DUCCI L., DOROSHENKO V., KOENIG O., BUCKLEY D.A.H., MONAGENG I.M., UDALSKI A.
	ATel, 3609, 1 (2020)
	eRASSU J050810.4-660653: SRG/eROSITA discovery of a new Be/X-ray binary in the LMC.
o	<eRASSU JHHMMSS.s+DDMMSS> N=1.
Ref:	=2020ATel13789....1H
by	HABERL F. , MAITRA C., GREINER J., CARPANO S., WILMS J., KREYKENBOHM I., WEBER P., KOENIG O., UDALSKI A.
	ATel, 3789, 1 (2020)
	SRG/eROSITA discovery of eRASSU J050213.8-674620, a candidate Be+WD X-ray binary system in the LMC.
o	<eRASSU JHHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ERC98]
[ERC98]	(Eck+Roberts+Cowan+, 1998)
Write:	<<[ERC98] HHMMSS.ss+DDMMSS.s>>
N:	1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	N=1 radio-source East of SN 1923A
Ref:	=1998ApJ...508..664E
by	ECK C.R. , ROBERTS D.A., COWAN J.J., BRANCH D.
	Astrophys. J., 508, 664-668 (1998)
	The probable detection of SN 1923A: the oldest radio supernova?.
o	Table 2: <[ERC98] 133420.18-293546.6> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ERE98]
[ERE98]	(Eyres+Richards+Evans+, 1998)
Write:	<<[ERE98] HHMMSS.sss+DDMMSS.ss>>
N:	8
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=8 confusing sources near V4334 Sgr.
Ref:	=1998MNRAS.297..905E
by	EYRES S.P.S. , RICHARDS A.M.S., EVANS A., BODE M.F.
	Mon. Not. R. Astron. Soc., 297, 905-909 (1998)
	Sakurai's object: the ionized nebula at radio wavelengths.
o	Table 1: <[ERE98] HHMMSS.sss-DDMMSS.ss> N=8
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ERG
ERG	(Extremely Red Galaxy)
*****	Avoid the usage of ERG, prefer [CDD99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ERG2015]
[ERG2015]	(Ellsworth-Bowers+Rosolowsky+Glenn+, 2015)= (BGPSv2)
Write:	<<[ERG2015] NNNN>>
N:	3508+1514
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	Submillimetric continuum observations of N=3508 molecular cloud clumps in the northern Galactic plane.
Ref:	=2015ApJ...799...29E
by	ELLSWORTH-BOWERS T.P. , ROSOLOWSKY E., GLENN J., GINSBURG A., EVANS II N.J., BATTERSBY C., SHIRLEY Y.L., SVOBODA B.
	Astrophys. J., 799, 29 (2015)
	The Bolocam Galactic Plane Survey. XII. Distance catalog expansion using kinematic isolation of dense molecular cloud structures with ^{13}CO(1-0).
o	Table 5: <[ERG2015] NNNN> N=3508 among (Nos 2216-8225).
Ref:	=2016ApJ...822...59S
by	SVOBODA B.E. , SHIRLEY Y.L., BATTERSBY C., ROSOLOWSKY E.W., GINSBURG A.G., ELLSWORTH-BOWERS T.P., PESTALOZZI M.R., DUNHAM M.K., EVANS II N.J., BALLY J., GLENN J.
	Astrophys. J., 822, 59-59 (2016)
	The Bolocam Galactic Plane Survey. XIV. Physical properties of massive starless and star-forming clumps.
o	Tables 3, 5-6: <[ERG2015] NNNN> N=1514 among (Nos 2351-7031) added.
=E=	Catalogue in electronic form as J/ApJ/799/29
=E=	Catalogue in electronic form as <J/ApJ/822/59/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ERK2011]
[ERK2011]	(Eger+Rowell+Kawamura+, 2011) (Not yet in Simbad)
Write:	<<[ERK2011] AN>>
N:	4
Object:	? + HII (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=2 absorption dips in HI and N=2 HII regions near HESS J1626-490.
Ref:	=2011A&A...526A..82E
by	EGER P. , ROWELL G., KAWAMURA A., FUKUI Y., ROLLAND L., STEGMANN C.
	Astron. Astrophys., 526A, 82-82 (2011)
	A multi-wavelength study of the unidentified TeV γ-ray source HESS J1626-490.
o	Figs 8-9: <[ERK2011] AN> (Nos D1-D2, R1-R2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ERL2020]
[ERL2020]	(Eppens+Reynoso+Lazendic-Galloway+, 2020)
Write:	<<[ERL2020] aN>>
N:	6
Object:	CO Clump (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	Kitt Peak Arizona Radio Observatory 12m radio telescope observations of N=6 CO clumps in SNR G359.1-00.5.
in source:	SNR G359.1-00.5
Ref:	=2020MNRAS.493.3947E
by	EPPENS L.K. , REYNOSO E.M., LAZENDIC-GALLOWAY J., COMBI J.A., ALBACETE-COLOMBO J.F.
	Mon. Not. R. Astron. Soc., 493, 3947-3955 (2020)
	Molecular environments of the supernova remnant G359.1-0.5.
o	Table 2: <[ERL2020] aN> (Nos a1-a2, b1, c1-c2, e1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ERO
ERO	(Extremely Red Object) (Not yet in Simbad)
*****	Avoid the usage of ERO, prefer [M2001]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ERO
ERO	(Extremely Red Object)
*****	Avoid the usage of ERO, prefer [DGI99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ERO
ERO	(Extremely Red Object)
*****	Avoid the usage of ERO, prefer [MCR2002]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ERO
ERO	(Extremely Red Object)
*****	Avoid the usage of ERO, prefer [MPW92]
Origin	of the Acronym: L (2000ApJ...533L..61G)
Details on Acronym: ERO
ERO	(Extremely Red Object)
*****	Avoid the usage of ERO, prefer [MRN2004b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ERO
ERO	(Extremely Red Object)
*****	Avoid the usage of ERO, prefer [MSK2003]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ERO
ERO	(Extremely Red Object)
*****	Avoid the usage of ERO, prefer [SOM2002]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ero
ero	(extremely red object)
*****	Avoid the usage of ero, prefer [SPI2003]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ERO
ERO	(Extremely Red Object)
*****	Avoid the usage of ERO, prefer [SSB2005b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ERO
ERO	(Extremely Red Object)
*****	Avoid the usage of ERO, prefer [SSK2002]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ERO
ERO	(Extremely Red Object)
*****	Avoid the usage of ERO, prefer [STE2001]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ERO
ERO	(Extremely Red Object)
*****	Avoid the usage of ERO, prefer [YMW2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EROS
EROS	(Experience de Recherche d'Objets Sombres)= (EROS1) = (EROS2)
Write:	<<EROS LMC NN>> <<EROS SMC NN>> <<EROS BLG YYYY NN>>
Object:	Microlensing Event (SIMBAD class: LensingEv = (Micro)Lensing Event)
Note:	Gravitational microlensing events in the LMC, the SMC, and the galactic Bulge (BLG in the format).
in source:	Magellanic Clouds:LMC = LMC
in source:	Magellanic Clouds:SMC = SMC
in source:	NAME Galactic Bulge
Ref:	=1993Natur.365..623A
by	AUBOURG E. , BAREYRE P., BREHIN S., GROS M., LACHIEZE-REY M., LAURENT B., LESQUOY E., MAGNEVILLE C., MILSZTAJN A., MOSCOSO L., QUEINNEC F., RICH J., SPIRO M., VIGROUX L., ZYLBERAJCH S., ANSARI R., CAVALIER F., MONIEZ M., BEAULIEU J.P., FERLET R., GRISON P., VIDAL-MADJAR A., GUIBERT J., MOREAU O., TAJAHMADY F., MAURICE E., PREVOT L., GRY C.
	Nature, 365, 623-625 (1993)
	Evidence for gravitational microlensing by dark objects in the Galactic halo.
o	Table 1: <EROS LMC N> (Nos 1-2).
Ref:	=1998A&A...332....1P
by	PALANQUE-DELABROUILLE N. , AFONSO C., ALBERT J.N., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., BAUER F., BEAULIEU J.P., BOUQUET A., CHAR S., CHARLOT X., COUCHOT F., COUTURES C., DERUE F., FERLET R., GLICENSTEIN J.F., GOLDMAN B., GOULD A., GRAFF D., GROS M., HAISSINSKI J., HAMILTON J.C., HARDIN D., DE KAT J., LESQUOY E., LOUP C., MAGNEVILLE C., MANSOUX B., MARQUETTE J.B., MAURICE E., MILSZTAJN A., MONIEZ M., PERDEREAU O., PREVOT L., RENAULT C., RICH J., SPIRO M., VIDAL-MADJAR A., VIGROUX L., ZYLBERAJCH S.
	Astron. Astrophys., 332, 1-9 (1998)
	Microlensing towards the Small Magellanic Cloud EROS 2 first year survey.
o	The EROS collaboration. p. 4: U0150-00676152 = USNO-A1.0 0150.00676152
o	Fig.3: <EROS SMC N> (No. 1).
Ref:	=2000A&A...355L..39L
by	LASSERRE T. , AFONSO C., ALBERT J.N., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., BAUER F., BEAULIEU J.P., BLANC G., BOUQUET A., CHAR S., CHARLOT X., COUCHOT F., COUTURES C., DERUE F., FERLET R., GLICENSTEIN J.F., GOLDMAN B., GOULD A., GRAFF D., GROS M., HAISSINSKI J., HAMILTON J.C., HARDIN D., DE KAT J., KIM A., LESQUOY E., LOUP C., MAGNEVILLE C., MANSOUX B., MARQUETTE J.B., MAURICE E., MILSZTAJN A., MONIEZ M., PALANQUE-DELABROUILLE N., PERDEREAU O., PREVOT L., REGNAULT N., RICH J., SPIRO M., VIDAL-MADJAR A., VIGROUX L., ZYLBERAJCH S.
	Astron. Astrophys., 355, 39-42 (2000)
	Not enough stellar mass Machos in the Galactic halo.
o	Table 1: <EROS LMC N> (Nos 3-4).
Ref:	=2001ApJ...548L.197C
by	CASTRO S. , POGGE R.W., RICH R.M., DEPOY D.L., GOULD A.
	Astrophys. J., 548, 197-200 (2001)
	Spatial/spectral resolution of a galactic bulge K3 giant stellar atmosphere via gravitational microlensing.
o	<EROS BLG 2000 N> (No. 5), 1st ref. with an EROS BLG object.
Ref:	=2003A&A...400..951A
by	AFONSO C. , ALBERT J.N., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., BEAULIEU J.P., BLANC G., CHARLOT X., COUCHOT F., COUTURES C., FERLET R., FOUQUE P., GLICENSTEIN J.F., GOLDMAN B., GOULD A., GRAFF D., GROS M., HAISSINSKI J., HAMADACHE C., DE KAT J., LASSERRE T., LE GUILLOU L., LESQUOY E., LOUP C., MAGNEVILLE C., MARQUETTE J.B., MAURICE E., MAURY A., MILSZTAJN A., MONIEZ M., PALANQUE-DELABROUILLE N., PERDEREAU O., PREVOT L., RAHAL Y.R., RICH J., SPIRO M., TISSERAND P., VIDAL-MADJAR A., VIGROUX L., ZYLBERAJCH S.
	Astron. Astrophys., 400, 951-956 (2003)
	Limits on Galactic dark matter with 5 years of EROS SMC data.
o	Table 1: <EROS SMC N> (Nos 2-4) added. Table 4: <EROS LMC N> (Nos 5-7) added.
Ref:	=2007A&A...469..387T
by	TISSERAND P. , LE GUILLOU L., AFONSO C., ALBERT J.N., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., BEAULIEU J.P., CHARLOT X., COUTURES C., FERLET R., FOUQUE P., GLICENSTEIN J.F., GOLDMAN B., GOULD A., GRAFF D., GROS M., HAISSINSKI J., HAMADACHE C., DE KAT J., LASSERRE T., LESQUOY E., LOUP C., MAGNEVILLE C., MARQUETTE J.B., MAURICE E., MAURY A., MILSZTAJN A., MONIEZ M., PALANQUE-DELABROUILLE N., PERDEREAU O., RAHAL Y.R., RICH J., SPIRO M., VIDAL-MADJAR A., VIGROUX L., ZYLBERAJCH S.
	Astron. Astrophys., 469, 387-404 (2007)
	Limits on the Macho content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds.
o	Table 2: <EROS SMC N> (No. 5) added, <EROS LMC NN> (Nos 8-12) added. Table 2, col(2): <EROS2-star smNNN-Na-NNNNN> N=2, <EROS2-star lmNNN-Na-NNNNN> N=5.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EROS
EROS	(Experience de Recherche d'Objets Sombres)
Write:	<<EROS NNNN>>
N:	79+97
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	1st ref.: EB* in the LMC, (Nos 1001-1079). Identif. charts. 2nd ref.: V* in the LMC, (Nos 2001-2097). Identif. charts. This is the final numbering in the LMC in the EROS catalogue. Results for SMC will be published, see [BKS97].
in source:	Magellanic Clouds:LMC = LMC
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1995A&AS..109..447G
by	GRISON P. , BEAULIEU J.-P., PRITCHARD J.D., TOBIN W., FERLET R., VIDAL-MADJAR A., GUIBERT J., ALARD C., MOREAU O., TAJAHMADY F., MAURICE E., PREVOT L., GRY C., AUBOURG E., BAREYRE P., BREHIN S., GROS M., LACHIEZE-REY M., LAURENT B., LESQUOY E., MAGNEVILLE C., MILSZTAJN A., MOSCOSO L., QUEINNEC F., RENAULT C., RICH J., SPIRO M., VIGROUX L., ZYLBERAJCH S., ANSARI R., CAVALIER F., MONIEZ M.
	Astron. Astrophys., Suppl. Ser., 109, 447-469 (1995)
	EROS catalogue of eclipsing binary stars in the bar of the Large Magellanic Cloud.
o	<EROS NNNN> (Nos 1001-1079), N=79
Ref:	=1995A&A...303..137B
by	BEAULIEU J.P. , GRISON P., TOBIN W., PRITCHARD J.D., FERLET R., LEPEINTRE F., VIDAL-MADJAR A., MAURICE E., PREVOT L., GRY C., GUIBERT J., MOREAU O., TAJHAMADY F., AUBOURG E., BAREYRE P., COUTURES C., GROS M., LAURENT B., LACHIEZE-REY M., LESQUOY E., MAGNEVILLE C., MILSZTAJN A., MOSCOSO L., QUEINNEC F., RENAULT C., RICH J., SPIRO M., VIGROUX L., ZYLBERAJCH S., ANSARI R., CAVALIER F., MONIEZ M.
	Astron. Astrophys., 303, 137-154 (1995)
	EROS variable stars: fundamental-mode and first-overtone Cepheids in the bar of the Large Magellanic Cloud.
o	<EROS NNNN> (Nos 2001-2097)
=E=	Catalogue in electronic form as J/A+AS/109/447
=E=	Catalogue in electronic form as J/A+A/303/137
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EROS ELHC
EROS ELHC	(EROS, LMC, HAeBe Candidate)
*****	Avoid the usage of EROS ELHC, prefer ELHC
Origin	of the Acronym: L (2000A&AS..145...11M)
Details on Acronym: EROS-2
EROS-2	(Experience de Recherche d'Objets Sombres)
*****	Avoid the usage of EROS-2, prefer EROS2
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EROS-BLG
EROS-BLG	(EROS, Gal. Bulge)
Write:	<<EROS2-BLG NN>>
Object:	Lensing Event (SIMBAD class: LensingEv = (Micro)Lensing Event)
Ref:	=2003A&A...404..145A
by	AFONSO C. , ALBERT J.N., ALARD C., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., BAUER F., BEAULIEU J.P., BLANC G., BOUQUET A., CHAR S., CHARLOT X., COUCHOT F., COUTURES C., DERUE F., FERLET R., FOUQUE P., GLICENSTEIN J.F., GOLDMAN B., GOULD A., GRAFF D., GROS M., HAISSINSKI J., HAMADACHE C., HAMILTON J.C., HARDIN D., DE KAT J., KIM A., LASSERRE T., LE GUILLOU L., LESQUOY E., LOUP C., MAGNEVILLE C., MANSOUX B., MARQUETTE J.B., MAURICE E., MAURY A., MILSZTAJN A., MONIEZ M., PALANQUE-DELABROUILLE N., PERDEREAU O., PREVOT L., REGNAULT N., RICH J., SPIRO M., TISSERAND P., VIDAL-MADJAR A., VIGROUX L., ZYLBERAJCH S.
	Astron. Astrophys., 404, 145-156 (2003)
	Bulge microlensing optical depth from EROS 2 observations.
o	These are EROS2 observations and thus they are called EROS2-BLG NN in Simbad and not EROS-BLG NN as proposed by the authors in the article. objects OGLE = EWS YYYY-AAA-NN, EROS YY-BLG NN = EROS BLG YYYY NN in Simbad.
o	Table 3: <[AAA2003] NN> (Nos 1-16) = <EROS2-BLG NN> N=16 among (Nos 2-35).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EROS-MP
EROS-MP	(Experience de Recherche d'Objets Sombres, Mouvement Propre)
Write:	<<EROS-MP JHHMM+DDMM>>
Object:	* (SIMBAD class: Star)
Note:	1999A&A...351L...5G: 1st ref. with an 'EROS-MP' object. L dwarfs from EROS 2, DENIS complementary observations.
Ref:	=1999A&A...351L...5G
by	GOLDMAN B. , DELFOSSE X., FORVEILLE T., AFONSO C., ALARD C., ALBERT J.N., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., BAUER F., BEAULIEU J.P., BORSENBERGER J., BOUQUET A., CHAR S., CHARLOT X., COUCHOT F., COUTURES C., DERUE F., FERLET R., FOUQUE P., GLICENSTEIN J.F., GOULD A., GRAFF D., GROS M., HAISSINSKI J., HAMILTON J.C., HARDIN D., DE KAT J., KIM A., LASSERRE T., LESQUOY E., LOUP C., MAGNEVILLE C., MANSOUX B., MARQUETTE J.B., MARTIN E.L., MAURICE E., MILSZTAJN A., MONIEZ M., PALANQUE-DELABROUILLE N., PERDEREAU O., PREVOT L., REGNAULT N., RICH J., SPIRO M., VIDAL-MADJAR A., VIGROUX L., ZYLBERAJCH S., (The EROS Collaboration)
	Astron. Astrophys., 351, 5-9 (1999)
	EROS 2 proper motion survey: a field brown dwarf, and an L dwarf companion to LHS 102.
o	<EROS-MP JHHMM+DDMM> N=1. <[GDF99] LHS 102B> N=1.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EROS1
EROS1	(Experience de Recherche d'Objets Sombres, phase 1)
*****	Avoid the usage of EROS1, prefer EROS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EROS2
EROS2	(Experience de Recherche d'Objets Sombres, phase 2)
*****	Avoid the usage of EROS2, prefer EROS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EROS2
EROS2	(Experience de Recherche d'Objets Sombres)
Write:	<<EROS2 FFF-N-N-NNNNN>>
N:	121
Object:	Lensing Event (SIMBAD class: LensingEv = (Micro)Lensing Event)
Note:	EROS-2 measurement of the microlensing optical depth toward the Galactic Bulge.
in source:	NAME Galactic Bulge
Ref:	=2006A&A...454..185H
by	HAMADACHE C. , LE GUILLOU L., TISSERAND P., AFONSO C., ALBERT J.N., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., BEAULIEU J.P., CHARLOT X., COUTURES C., FERLET R., FOUQUE P., GLICENSTEIN J.F., GOLDMAN B., GOULD A., GRAFF D., GROS M., HAISSINSKI J., DE KAT J., LESQUOY E., LOUP C., MAGNEVILLE C., MARQUETTE J.B., MAURICE E., MAURY A., MILSZTAJN A., MONIEZ M., PALANQUE-DELABROUILLE N., PERDEREAU O., RAHAL Y.R., RICH J., SPIRO M., VIDAL-MADJAR A., VIGROUX L., ZYLBERAJCH S.
	Astron. Astrophys., 454, 185-199 (2006)
	Galactic Bulge microlensing optical depth from EROS-2.
o	Table 3: <EROS2 FFF-N-N-NNNNN> N=121.
=E=	Catalogue in electronic form as J/A+A/454/185
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EROS2-BC
EROS2-BC	(EROS2-Beat Cepheid)
Write:	<<EROS2-BC JHHMMSS+DDMMSS>>
N:	414
Object:	Beat Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Stat:	is completely incorporated in Simbad
Note:	Beat Cepheids in the Magellanic Clouds from the EROS2 database. See also EROS2-star.
in source:	Magellanic Clouds: LMC = LMC
in source:	Magellanic Clouds: SMC = SMC
Ref:	=2009A&A...495..249M
by	MARQUETTE J.B. , BEAULIEU J.P., BUCHLER J.R., SZABO R., TISSERAND P., BELGHITH S., FOUQUE P., LESQUOY E., MILSZTAJN A., SCHWARZENBERG-CZERNY A., AFONSO C., ALBERT J.N., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., CHARLOT X., COUTURES C., FERLET R., GLICENSTEIN J.F., GOLDMAN B., GOULD A., GRAFF D., GROS M., HAIESSINSKI J., HAMADACHE C., DE KAT J., LE GUILLOU L., LOUP C., MAGNEVILLE C., MAURICE E., MAURY A., MONIEZ M., PALANQUE-DELABROUILLE N., PERDEREAU O., RAHAL Y.R., RICH J., SPIRO M., VIDAL-MADJAR A.
	Astron. Astrophys., 495, 249-256 (2009)
	The beat Cepheids in the Magellanic clouds: an analysis from the EROS-2 database.
o	Fig. 1, Text: <EROS2-star lmNNN-Na-NNNNN> N=9 added. Tables 1-4: <EROS2-BC JHHMMSS+DDMMSS> N=74+173+41+129.
=E=	Catalogue in electronic form as J/A+A/495/249
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EROS2-BLG
EROS2-BLG	(EROS2, Gal. Bulge)
Write:	<<EROS2-BLG NN>>
N:	16
Object:	Lensing Event (SIMBAD class: LensingEv = (Micro)Lensing Event)
Note:	EROS 2 observations of the Galactic Bulge searching for microlensing event candidates. See also [AAA2003].
Ref:	=2003A&A...404..145A
by	AFONSO C. , ALBERT J.N., ALARD C., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., BAUER F., BEAULIEU J.P., BLANC G., BOUQUET A., CHAR S., CHARLOT X., COUCHOT F., COUTURES C., DERUE F., FERLET R., FOUQUE P., GLICENSTEIN J.F., GOLDMAN B., GOULD A., GRAFF D., GROS M., HAISSINSKI J., HAMADACHE C., HAMILTON J.C., HARDIN D., DE KAT J., KIM A., LASSERRE T., LE GUILLOU L., LESQUOY E., LOUP C., MAGNEVILLE C., MANSOUX B., MARQUETTE J.B., MAURICE E., MAURY A., MILSZTAJN A., MONIEZ M., PALANQUE-DELABROUILLE N., PERDEREAU O., PREVOT L., REGNAULT N., RICH J., SPIRO M., TISSERAND P., VIDAL-MADJAR A., VIGROUX L., ZYLBERAJCH S.
	Astron. Astrophys., 404, 145-156 (2003)
	Bulge microlensing optical depth from EROS 2 observations.
o	These are EROS2 observations and thus they are called EROS2-BLG NN in Simbad and not EROS-BLG NN as proposed by the authors in the article. objects OGLE = EWS YYYY-AAA-NN, EROS YY-BLG NN = EROS BLG YYYY NN in Simbad.
o	Table 3: <[AAA2003] NN> (Nos 1-16) = <EROS2-BLG NN> N=16 among (Nos 2-35).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EROS2-GSA
EROS2-GSA	(Exper. de Recherche d'Objets Sombres, II, Gal. Spiral Arm)
Write:	<<EROS2-GSA NN>> <<EROS2-GSA uN>>
N:	30+1
Object:	Poss. Microlensing Event (SIMBAD class: LensingEv = (Micro)Lensing Event)
Note:	Microlensing events towards the Galactic spiral arms.
Ref:	=1999A&A...351...87D
by	DERUE F. , AFONSO C., ALARD C., ALBERT J.N., AMADON A., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., BAUER F., BEAULIEU J.-P., BOUQUET A., CHAR S., CHARLOT X., COUCHOT F., COUTURES C., FERLET R., GLICENSTEIN J.-F., GOLDMAN B., GOULD A., GRAFF D., GROS M., HAISSINSKI J., HAMILTON J.C., HARDIN D., DE KAT J., KIM A., LASSERRE T., LESQUOY E., LOUP C., MAGNEVILLE C., MANSOUX B., MARQUETTE J.-B., MAURICE E., MILSZTAJN A., MONIEZ M., PALANQUE-DELABROUILLE N., PERDEREAU O., PREVOT L., REGNAULT N., RICH J., SPIRO M., VIDAL-MADJAR A., VIGROUX L., ZYLBERAJCH S., (The EROS Collaboration)
	Astron. Astrophys., 351, 87-96 (1999)
	Observation of microlensing towards the galactic spiral arms. EROS II. 2 year survey.
o	Table 2: <EROS2-GSA N> (Nos 1-3).
Ref:	=2001A&A...373..126D
by	DERUE F. , AFONSO C., ALARD C., ALBERT J.N., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., BAUER F., BEAULIEU J.-P., BLANC G., BOUQUET A., CHAR S., CHARLOT X., COUCHOT F., COUTURES C., FERLET R., FOUQUE P., GLICENSTEIN J.-F., GOLDMAN B., GOULD A., GRAFF D., GROS M., HAISSINSKI J., HAMILTON J.C., HARDIN D., DE KAT J., KIM A., LASSERRE T., LE GUILLOU L., LESQUOY E., LOUP C., MAGNEVILLE C., MANSOUX B., MARQUETTE J.-B., MAURICE E., MILSZTAJN A., MONIEZ M., PALANQUE-DELABROUILLE N., PERDEREAU O., PREVOT L., REGNAULT N., RICH J., SPIRO M., VIDAL-MADJAR A., VIGROUX L., ZYLBERAJCH S.
	Astron. Astrophys., 373, 126-138 (2001)
	Observation of microlensing toward the galactic spiral arms. EROS II 3 year survey.
o	Table 3: <EROS2-GSA N> (Nos 4-7) added.
Ref:	=2009A&A...500.1027R
by	RAHAL Y.R. , AFONSO C., ALBERT J.-N., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., BEAULIEU J.-P., CHARLOT X., COUCHOT F., COUTURES C., DERUE F., FERLET R., FOUQUE P., GLICENSTEIN J.-F., GOLDMAN B., GOULD A., GRAFF D., GROS M., HAIESSINSKI J., HAMADACHE C., DE KAT J., LESQUOY E., LOUP C., LE GUILLOU L., MAGNEVILLE C., MANSOUX B., MARQUETTE J.-B., MAURICE E., MAURY A., MILSZTAJN A., MONIEZ M., PALANQUE-DELABROUILLE N., PERDEREAU O., RAHVAR S., RICH J., SPIRO M., TISSERAND P., VIDAL-MADJAR A., (The EROS-2 Collaboration)
	Astron. Astrophys., 500, 1027-1044 (2009)
	The EROS2 search for microlensing events towards the spiral arms: the complete seven season results.
o	Table 2: <EROS2-GSA NN> (Nos 8-30) added, <EROS2-GSA uN> (No. u1).
=E=	Catalogue in electronic form as <J/A+A/500/1027/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EROS2-GSA
EROS2-GSA	(Exper. de Recherche d'Objets Sombres, II, Gal. Spiral Arm)
Write:	<<EROS2-GSA JHHMMSS+DDMMSS>>
N:	431+928
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	Search for variable stars by EROS II. N=431 variable with periods lower than 30 days and N=930 with periods greater than 30 days.
Ref:	=2002A&A...389..149D
by	DERUE F. , MARQUETTE J.-B., LUPONE S., AFONSO C., ALARD C., ALBERT J.-N., AMADON A., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., BAUER F., BEAULIEU J.-P., BLANC G., BOUQUET A., CHAR S., CHARLOT X., COUCHOT F., COUTURES C., FERLET R., FOUQUE P., GLICENSTEIN J.-F., GOLDMAN B., GOULD A., GRAFF D., GROS M., HAIESSINSKI J., HAMILTON J.-C., HARDIN D., DE KAT J., KIM A., LASSERRE T., LE GUILLOU L., LESQUOY E., LOUP C., MAGNEVILLE C., MANSOUX B., MAURICE E., MILSZTAJN A., MONIEZ M., PALANQUE-DELABROUILLE N., PERDEREAU O., PREVOT L., REGNAULT N., RICH J., SPIRO M., VIDAL-MADJAR A., VIGROUX L., ZYLBERAJCH S., (The EROS Collaboration)
	Astron. Astrophys., 389, 149-161 (2002)
	Observation of periodic variable stars towards the Galactic spiral arms by EROS. II.
o	Tables 3, 4: <EROS2-GSA JHHMMSS+DDMMSS> N=431+928.
=E=	Catalogue in electronic form as J/A+A/389/149
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EROS2-star
EROS2-star	(Experience de Recherche d'Objets Sombres, 2, star)
Write:	<<EROS2-star aaNNN-Na-NNNNN>> <<EROS2-star aaNNNNaNNNNN>>
N:	40
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	EROS2 bright star different format designations in literature. See also [TMW2008].
Ref:	=2007A&A...469..387T
by	TISSERAND P. , LE GUILLOU L., AFONSO C., ALBERT J.N., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., BEAULIEU J.P., CHARLOT X., COUTURES C., FERLET R., FOUQUE P., GLICENSTEIN J.F., GOLDMAN B., GOULD A., GRAFF D., GROS M., HAISSINSKI J., HAMADACHE C., DE KAT J., LASSERRE T., LESQUOY E., LOUP C., MAGNEVILLE C., MARQUETTE J.B., MAURICE E., MAURY A., MILSZTAJN A., MONIEZ M., PALANQUE-DELABROUILLE N., PERDEREAU O., RAHAL Y.R., RICH J., SPIRO M., VIDAL-MADJAR A., VIGROUX L., ZYLBERAJCH S.
	Astron. Astrophys., 469, 387-404 (2007)
	Limits on the Macho content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds.
o	Table 2: <EROS SMC N> (No. 5) added, <EROS LMC NN> (Nos 8-12) added. Table 2, col(2): <EROS2-star smNNN-Na-NNNNN> N=2, <EROS2-star lmNNN-Na-NNNNN> N=5.
Ref:	=2008A&A...481..673T
by	TISSERAND P. , MARQUETTE J.B., WOOD P.R., LESQUOY E., BEAULIEU J.P., MILSZTAJN A., HAMADACHE C., AFONSO C., ALBERT J.N., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., CHARLOT X., COUTURES C., FERLET R., FOUQUE P., GLICENSTEIN J.F., GOLDMAN B., GOULD A., GROS M., HAISSINSKI J., DE KAT J., LE GUILLOU L., LOUP C., MAGNEVILLE C., MAURICE E., MAURY A., MONIEZ M., PALANQUE-DELABROUILLE N., PERDEREAU O., RAHAL Y., RICH J., SPIRO M., VIDAL-MADJAR A., ZYLBERAJCH S.
	Astron. Astrophys., 481, 673-690 (2008)
	R Coronae Borealis stars in the Galactic bulge discovered by EROS-2.
o	Table 3, col(1): <[TMW2008] EROS2-GC-RCB-NN> (Nos 01-14). Table 3, col(2), Table 4, col(1): <EROS2-star cgNNNNaNNNNN> N=14+9.
Ref:	=2008A&A...486..891M
by	MARQUETTE J.B. , TISSERAND P., FRANCOIS P., BEAULIEU J.P., DOUBLIER V., LESQUOY E., MILSZTAJN A., PRITCHARD J., SCHWARZENBERG-CZERNY A., AFONSO C., ALBERT J.N., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., CHARLOT X., COUTURES C., FERLET R., FOUQUE P., GLICENSTEIN J.F., GOLDMAN B., GOULD A., GRAFF D., GROS M., HAISSINSKI J., HAMADACHE C., DE KAT J., LE GUILLOU L., LOUP C., MAGNEVILLE C., MAURICE E., MAURY A., MONIEZ M., PALANQUE-DELABROUILLE N., PERDEREAU O., RAHAL Y.R., RICH J., SPIRO M., VIDAL-MADJAR A., ZYLBERAJCH S.
	Astron. Astrophys., 486, 891-898 (2008)
	Discovery of a peculiar Cepheid-like star towards the northern edge of the Small Magellanic Cloud.
o	EROS2 J005135-714459 = EROS2-star sm006-0n-13842
o	Fig.2: <EROS2-star smNNN-Na-NNNNN> N=1 added.
Ref:	=2009A&A...495..249M
by	MARQUETTE J.B. , BEAULIEU J.P., BUCHLER J.R., SZABO R., TISSERAND P., BELGHITH S., FOUQUE P., LESQUOY E., MILSZTAJN A., SCHWARZENBERG-CZERNY A., AFONSO C., ALBERT J.N., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., CHARLOT X., COUTURES C., FERLET R., GLICENSTEIN J.F., GOLDMAN B., GOULD A., GRAFF D., GROS M., HAIESSINSKI J., HAMADACHE C., DE KAT J., LE GUILLOU L., LOUP C., MAGNEVILLE C., MAURICE E., MAURY A., MONIEZ M., PALANQUE-DELABROUILLE N., PERDEREAU O., RAHAL Y.R., RICH J., SPIRO M., VIDAL-MADJAR A.
	Astron. Astrophys., 495, 249-256 (2009)
	The beat Cepheids in the Magellanic clouds: an analysis from the EROS-2 database.
o	Fig. 1, Text: <EROS2-star lmNNN-Na-NNNNN> N=9 added. Tables 1-4: <EROS2-BC JHHMMSS+DDMMSS> N=74+173+41+129.
=E=	Catalogue in electronic form as <J/A+A/486/891/>
=E=	Catalogue in electronic form as <J/A+A/495/249/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ERR88]
[ERR88]	(Elston+Rieke+Rieke, 1988)
Write:	<<[ERR88] HHMMSS.ss+DDMMSS.s>>
N:	4
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Ref:	=1988ApJ...331L..77E
by	ELSTON R. , RIEKE G.H., RIEKE M.J.
	Astrophys. J., 331, 77-80 (1988)
	Deep 2 micron imaging of the sky: evidence for a new extragalactic population.
o	Table 1: <[ERR88] HHMMSS.ss+DDMMSS.s> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ERS
ERS	(Early Science Release)
*****	Avoid the usage of ERS, prefer [HZR2011]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ERS2021]
[ERS2021]	(Beling+Richard+Smail+, 2021)
Write:	<<[ERS2021] eMACS J0252 N>> <<[ERS2021] eMACS J0252 Na.N>> <<[ERS2021] eMACS J0252 BCG>> <<[ERS2021] JHHMMSS.ss+DDMMSS.s>>
N:	9+3+1+87
Object:	Grav. lensed image of a G + BCG + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Gemini-North GMOS and VLT MUSE observations of N=9 gravitationally lensed images in N=3 multiply-imaged systems lensed by the galaxy cluster eMACS J0252.4-2100, N=1 brightest galaxy and N=87 galaxies in the field of eMACS J0252.4-2100.
in source:	SPT-CL J0252-2100 = eMACS J0252.4-2100
Ref:	=2021MNRAS.508.3663E
by	EBELING H. , RICHARD J., SMAIL I., EDGE A.C., KOEKEMOER A.M., ZALESKY L.
	Mon. Not. R. Astron. Soc., 508, 3663-3671 (2021)
	An extreme case of galaxy and cluster co-evolution at z = 0.7.
o	Fig. 1, Table 1: <[ERS2021] eMACS J0252 Na.N> (Nos 1.1-1.3, 1a.1-1a.3, 2.1-2.3). Section 3.2.1: <[ERS2021] eMACS J0252 BCG> N=1. Table A1: <[ERS2021] JHHMMSS.ss+DDMMSS.s> N=87.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ERSO
ERSO	(Extremely Red Stellar Object)
*****	Avoid the usage of ERSO, prefer [WGB2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ERSy
ERSy	(Early Release Science y)
*****	Avoid the usage of ERSy, prefer [LBG2010]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ERW69]
[ERW69]	(Ellder+Ronnang+Winnberg, 1969)
Write:	<<[ERW69] N>>
N:	4
Object:	OH Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
in source:	NAME Cyg Region
Ref:	=1969Natur.222...67E
by	ELLDER J. , RONNANG B., WINNBERG A.
	Nature, 222, 67-69 (1969)
	New OH radio emission sources in Cygnus.
o	Table 1: <[ERW69] N> (Nos 1-4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ERX
ERX	(ER Eri region, (RX))
*****	Avoid the usage of ERX, prefer [TDQ2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 0ES
0ES	(Einstein Slew survey, version No. 0)
Write:	<<0ES HHMM+DD.d>>
N:	235
Object:	(X) (SIMBAD class: X = X-ray Source)
Ref:	=1994HEAO2.C......0M
by	McDOWELL J.C.
	Einstein Obs. Unscreened IPC Data Archive, 0-None (1994)
	The Einstein Observatory Soft X-ray Source List.
o	SAO HEAD CD-ROM Series I (Einstein), Nos 18-36
o	<2E HHMM.m+DDMM>, <2E NNNN>, <0ES HHMM+DD.d>.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 1ES
1ES	(Einstein Slew survey, version No. 1)
Write:	<<1ES HHMM+DD.dA>>
N:	821
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Ref:	=1992ApJS...80..257E
by	ELVIS M. , PLUMMER D., SCHACHTER J., FABBIANO G.
	Astrophys. J., Suppl. Ser., 80, 257-303 (1992)
	The Einstein Slew Survey.
o	Table 6: <1ES HHMM+DD.dA> N=821.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ES2000]
[ES2000]	(Evans+Seward, 2000)
Write:	<<[ES2000] NN>>
N:	26
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations.
in source:	NAME h Per = NGC 869
in source:	NAME khi Per = NGC 884
Ref:	=2000ApJ...538..777E
by	EVANS N.R. , SEWARD F.D.
	Astrophys. J., 538, 777-782 (2000)
	Settling onto the main sequence: ROSAT observations of h and χ Persei.
o	Table 1: <[ES2000] NN> (Nos 1-26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ES94]
[ES94]	(Elson+Schade, 1994)
Write:	<<[ES94] R-NN>>
N:	24
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Stat:	is completely incorporated in Simbad
Note:	In the format, the roman digit stands for 4 chips (Nos I to IV). Chip I: N=3, Chip II: N=10, Chip III: N=5, Chip IV: N=6. Observations from HST, WFC.
in source:	NAME Fornax Cluster
Ref:	=1994ApJ...437..625E
by	ELSON R.A.W. , SCHADE D.J.
	Astrophys. J., 437, 625-629 (1994)
	Structural parameters of globular clusters in the Fornax cluster.
o	Table 1: <[ES94] R-NN> N=24
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ESB2004]
[ESB2004]	(Eisenhardt+Stern+Brodwin+, 2004)= (IRAC)
Write:	<<[ESB2004] IRAC JHHMMSS.s+DDMMSS>>
N:	1
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	IRAC shallow survey of the NOAO Deep field in Bootes. See also [SEB2005], [BBA2006].
in source:	NAME Bootes Field
Ref:	=2004ApJS..154...48E
by	EISENHARDT P.R. , STERN D., BRODWIN M., FAZIO G.G., RIEKE G.H., RIEKE M.J., WERNER M.W., WRIGHT E.L., ALLEN L.E., ARENDT R.G., ASHBY M.L.N., BARMBY P., FORREST W.J., HORA J.L., HUANG J.-S., HUCHRA J., PAHRE M.A., PIPHER J.L., REACH W.T., SMITH H.A., STAUFFER J.R., WANG Z., WILLNER S.P., BROWN M.J.I., DEY A., JANNUZI B.T., TIEDE G.P.
	Astrophys. J., Suppl. Ser., 154, 48-53 (2004)
	The Infrared Array Camera (IRAC) shallow survey.
o	Fig.6: <[ESB2004] IRAC JHHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ESC2002]
[ESC2002]	(Eracleous+Shields+Charta+, 2002)
Write:	<<[ESC2002] NGC 4736 X-N>> <<[ESC2002] NGC 4579 X-N>>
N:	4+1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of NGC 4736 and NGC 4579.
in source:	NGC 4736
in source:	NGC 4579
Ref:	=2002ApJ...565..108E
by	ERACLEOUS M. , SHIELDS J.C., CHARTAS G., MORAN E.C.
	Astrophys. J., 565, 108-124 (2002)
	Three LINERs under the Chandra X-ray microscope.
o	Table 4: <[ESC2002] NGC 4736 X-N> (Nos X-1 to X-4). Table 5: <[ESC2002] NGC 4579 X-N> (No. X-1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ESC2021]
[ESC2021]	(Endsley+Stark+Chevallard+, 2021)= ([ESC2021a])
Write:	<<[ESC2021] COS-NNNNNNN>> <<[ESC2021] XMM1-NNNNNN>> <<[ESC2021] GW-NNNNN>>
N:	41+9+38+15
Object:	G (SIMBAD class: Galaxy)
Note:	N=41+9+38+15 z∼7 sourcecandidates in the COSMOS, XMM, GOODS-S, and GOODS-N fields respectively. Use of HST and Spitzer IRAC data and of data from previous surveys (like VIDEO, HSCSSP, UKIDSS, UltraVISTA). See also [ESC2021b].
Ref:	=2021MNRAS.500.5229E
by	ENDSLEY R. , STARK D.P., CHEVALLARD J., CHARLOT S.
	Mon. Not. R. Astron. Soc., 500, 5229-5248 (2021)
	The [O III]+H β equivalent width distribution at z ≃ 7: implications for the contribution of galaxies to reionization.
o	Table 1: <[ESC2021] COS-NNNNNNN> N=41 among (Nos 83688-1387948), <[ESC2021] XMM1-NNNNNN> N=9 among (Nos 88011-426118). Table 2: <[ESC2021] GN-NNNNN> N=15 among (Nos 2781-67013) N=38 among (Nos 2781-67013), <[ESC2021] GS-NNNNN> N=15 among (Nos 897-42630).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ESC2021a]
[ESC2021a]	(Endsley+Stark+Chevallard+, 2021)
*****	Avoid the usage of [ESC2021a], prefer [ESC2021]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ESC2021b]
[ESC2021b]	(Endsley+Stark+Charlot+, 2021)
Write:	<<[ESC2021b] COS-NNNNNNN>> <<[ESC2021b] XMM3-NNNNNN>>
N:	30+5
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	MMT Binospec observations of N=22 galaxies at z∼7 in the COSMOS and XMM fields. See also [ESC2021].
Ref:	=2021MNRAS.502.6044E
by	ENDSLEY R. , STARK D.P., CHARLOT S., CHEVALLARD J., ROBERTSON B., BOUWENS R.J., STEFANON M.
	Mon. Not. R. Astron. Soc., 502, 6044-6063 (2021)
	MMT spectroscopy of Lyman-α at z ≃ 7: evidence for accelerated reionization around massive galaxies.
o	Tables 2+4: <[ESC2021b] COS-NNNNNNN> N=20+10 among (Nos 221419-1260899), <[ESC2021b] XMM3-NNNNN> N=2+3 among (Nos 198954-569712).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Escorial
Escorial	(El Escorial)
Write:	<<Escorial NN>>
N:	35
Object:	Agglomerate (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Study of the spatial structure of regions rich in Hipparcos stars with B(T)-V(T) colours. See also [CD2008].
Ref:	=2008AN....329..801C
by	CABALLERO J.A. , DINIS L.
	AN, 329, 801-834 (2008)
	A revisit to agglomerate of early-type Hipparcos stars.
o	Table 1: <Escorial NN> (Nos 1-35). Table 3: <[CD2008] R> (Nos I to XXI).
=E=	Catalogue in electronic form as <J/AN/329/801/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ESD96]
[ESD96]	(Eisloffel+Smith+Davis+, 1996)
Write:	<<[ESD96] WN>> <<[ESD96] WA>>
N:	6+8
Object:	Bow + Knot (SIMBAD class: PartofCloud = Part of Cloud)
Note:	Calar Alto observations. Tables 1, 2: N=6 bows in Cep E, map in Fig. 1 (Plate 99). Table 3: N=8 knots in Cep E, map in Fig. 2 (Plate 101)
in source:	NAME Cep E
Ref:	=1996AJ....112.2086E
by	EISLOEFFEL J. , SMITH M.D., DAVIS C.J., RAY T.P.
	Astron. J., 112, 2086-2093 (1996)
	Molecular hydrogen in the outflow from Cep E.
o	Tables 1, 2: <[ESD96] WN> (Nos N1-N3, W1-W2, S1). Table 3: <[ESD96] WA> (Nos NA-NE, SA-SC)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ESDO
ESDO	(Eder+Schombert+Dekel+Oemler)
Write:	<<ESDO FFF-NN>> <<ESDO HHMMSS.s+DDMMSS>>
N:	466
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Dwarf galaxies in POSS fields (FFF in the format). In paper 1997ApJS..111..233S galaxies are not numbered, but found numbered in the literature.
Ref:	=1989ApJ...340...29E
by	EDER J.A. , SCHOMBERT J.M., DEKEL A., OEMLER A.
	Astrophys. J., 340, 29-46 (1989)
	The clustering of dwarf galaxies.
o	in ref list IKEUCHI 1981PASJ.33.211 instead of 221
o	Table 2: <ESDO HHMMSS.s+DDMMSS> = <ESDO FFF-NN>, N=178.
Ref:	=1997ApJS..111..233S
by	SCHOMBERT J.M. , PILDIS R.A., EDER J.A.
	Astrophys. J., Suppl. Ser., 111, 233-244 (1997)
	Gas-rich dwarfs from the second Palomar sky survey. I. Catalog and characteristics.
o	Table 1: <ESDO FFF-NN> N=278.
Ref:	=2000ApJS..131...47E
by	EDER J.A. , SCHOMBERT J.M.
	Astrophys. J., Suppl. Ser., 131, 47-70 (2000)
	Gas-rich dwarfs from the PSS-II. III. H I profiles and dynamical masses.
o	Table 1: <ESDO FFF-NN> N=393.
=E=	Catalogue in electronic form as J/ApJS/131/47
Origin	of the Acronym: L (1998ApJS..119..159S)
Details on Acronym: [ESE2014]
[ESE2014]	(Ebeling+Stephenson+Edge, 2014)
Write:	<<[ESE2014] MACSJHHMM-JFGNA>> <<[ESE2014] RXJ2248-JFG1>>
N:	6+9
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Identification of N=6 jellyfish galaxies in X-ray selected clusters at z>0.3 from MACS and CLASH surveys. Use of archival HST ACS images.
Ref:	=2014ApJ...781L..40E
by	EBELING H. , STEPHENSON L.N., EDGE A.C.
	Astrophys. J., 781L, 40 (2014)
	Jellyfish: evidence of extreme ram-pressure stripping in massive galaxy clusters.
o	Table 1: <[ESE2014] MACSJHHMM-JFG1> N=6.
Ref:	=2016MNRAS.455.2994M
by	McPARTLAND C. , EBELING H., ROEDIGER E., BLUMENTHAL K.
	Mon. Not. R. Astron. Soc., 455, 2994-3008 (2016)
	Jellyfish: the origin and distribution of extreme ram-pressure stripping events in massive galaxy clusters.
o	Table 1 : second occurence of MACSJ0429-JFG1 named MACSJ0429-JFG2 in SIMBAD; second occurence of MACSJ1752-JFG1 named MACSJ1752-JFG2 in SIMBAD.
o	Table 1: <[ESE2014] MACSJHHMM-JFGN> N=8 added, <[ESE2014] RXJHHMM-JFG1> N=1 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ESG
ESG	(Elson+Santiago+Gilmore)
Write:	<<ESG Red N>> <<ESG Blue NN>> <<ESG G>>
N:	9+50+1
Object:	* + G (SIMBAD class: Star)
Note:	Unresolved objects in the HDF. Table 1, Fig.4a: N=9 redder objects. Table 2, Fig.4b, c: N=50 faint blue objects. Fig.7 shows a bright elliptical galaxy, format 'G'. The 17 GlCl candidates are not numbered by the authors, so they are not included in SIMBAD.
in source:	NAME HDFN
Ref:	=1996NewA....1....1E
by	ELSON R.A.W. , SANTIAGO B.X., GILMORE G.F.
	New Astronomy, 1, 1-16 (1996)
	Halo stars, starbursts, and distant globular cluster: A survey of unresolved objects in the Hubble Deep Field.
o	Table 1, Fig.4a: <ESG Red N> (Nos 1-9). Table 2, Fig.4b,c: <ESG Blue NN> (Nos 1-50). Fig.7: <ESG G> N=1.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: ESHC
ESHC	(EROS, SMC, HAeBe Candidate)
Write:	<<ESHC N>>
N:	7
Object:	PMS* (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	EROS 2 SMC observations. See also ELHC.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2001A&A...380..168B
by	BEAULIEU J.-P. , DE WIT W.J., LAMERS H.J.G.L.M., MARQUETTE J.-B., COUTURES C., LEISY P., TOTOR S., PALANQUE-DELABROUILLE N., AFONSO C., ALARD C., ALBERT J.N., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., BAUER F., BLANC G., CHARLOT X., COUCHOT F., DERUE F., FERLET R., FOUQUE P., GLICENSTEIN J.-F., GOLDMAN B., GRAFF D., GROS M., HAISSINSKI J., HAMILTON J.C., HARDIN D., DE KAT J., LASSERRE T., LESQUOY E., LOUP C., MAGNEVILLE C., MANSOUX B., MAURICE E., MILSZTAJN A., MONIEZ M., PERDEREAU O., PREVOT L., REGNAULT N., RICH J., SPIRO M., VIDAL-MADJAR A., VIGROUX L., ZYLBERAJCH S.
	Astron. Astrophys., 380, 168-176 (2001)
	Blue irregular variable stars in the Small Magellanic Cloud from EROS2: Herbig Ae/Be or classical Be stars?
o	Table 1: <ESHC N> (Nos 1-2).
Ref:	=2003A&A...410..199D
by	DE WIT W.J. , BEAULIEU J.-P., LAMERS H.J.G.L.M., LESQUOY E., MARQUETTE J.-B.
	Astron. Astrophys., 410, 199-216 (2003)
	A quest for PMS candidate stars at low metallicity: Variable HAe/Be and Be stars in the Small Magellanic Cloud.
o	Table 3: <ESHC N> (Nos 3-7) added.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ESIS
ESIS	(ESO-Spitzer extragalactic Imaging Survey)
Write:	<<ESIS NNNNNN>> <<ESIS JHHMMSS.ss+DDMMSS.ss>>
N:	132612
Object:	G (SIMBAD class: Galaxy)
Note:	The ESO-Spitzer extragalactic Imaging Survey is the optical follow up of the SWIRE survey in the ELAIS S1 area.
in source:	ELAIS S1
Ref:	=2006A&A...451..881B
by	BERTA S. , RUBELE S., FRANCESCHINI A., HELD E.V., RIZZI L., LONSDALE C.J., JARRETT T.H., RODIGHIERO G., OLIVER S.J., DIAS J.E., BUTTERY H.J., FIORE F., LA FRANCA F., PUCCETTI S., FANG F., SHUPE D., SURACE J., GRUPPIONI C.
	Astron. Astrophys., 451, 881-900 (2006)
	The ESO-Spitzer Imaging extragalactic Survey (ESIS). I. WFI B, V, R deep observations of ELAIS-S1 and comparison to Spitzer and GALEX data.
o	<ESIS NNNNNN> = <ESIS JHHMMSS.ss+DDMMSS.ss> N=132612.
Ref:	=2007A&A...476..151B
by	BERTA S. , LONSDALE C.J., POLLETTA M., SAVAGE R.S., FRANCESCHINI A., BUTTERY H., CIMATTI A., DIAS J., FERUGLIO C., FIORE F., HELD E.V., LA FRANCA F., MAIOLINO R., MARCONI A., MATUTE I., OLIVER S.J., RICCIARDELLI E., RUBELE S., SACCHI N., SHUPE D., SURACE J.
	Astron. Astrophys., 476, 151-175 (2007)
	The contribution of very massive high-redshift SWIRE galaxies to the stellar mass function.
o	Table: <ESIS NNNNNN> N=326 among (Nos 69900-264125).
Ref:	=2009ApJ...703.1778S
by	SACCHI N. , LA FRANCA F., FERUGLIO C., FIORE F., PUCCETTI S., COCCHIA F., BERTA S., BRUSA M., CIMATTI A., COMASTRI A., FRANCESCHINI A., GRUPPIONI C., MAIOLINO R., MATUTE I., POLLETTA M., POZZETTI L., POZZI F., VIGNALI C., ZAMORANI G., OLIVER S., ROWAN-ROBINSON M., SMITH G., LONSDALE C.
	Astrophys. J., 703, 1778-1790 (2009)
	Spectroscopic identifications of Spitzer sources in the SWIRE/XMM-Newton/ELAIS-S1 field: a large fraction of active galactic nucleus with high F(24 µm)/F(R) ratio.
o	Table 2: <ESIS JHHMMSS.ss+DDMMSS.ss> N=1376.
=E=	Catalogue in electronic form as J/A+A/451/881
=E=	Catalogue in electronic form as J/A+A/476/151
=E=	Catalogue in electronic form as J/A+A/703/1778
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ESK2001]
[ESK2001]	(Ellis+Santos+Knieb+, 2001)
Write:	<<[ESK2001] a>> <<[ESK2001] GN>>
N:	3+2
Object:	Grav. lensed image + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 images of the lensing cluster ACO 2218: N=3 Ly-alpha-emitting lensing images (Nos a-c) of a galaxyfound later as KESR Galaxy. N=2 galaxies (Nos G1-G2).
in source:	ACO 2218
Ref:	=2001ApJ...560L.119E
by	ELLIS R. , SANTOS M.R., KNEIB J.-P., KUIJKEN K.
	Astrophys. J., 560, 119-122 (2001)
	A faint star-forming system viewed through the lensing cluster Abell 2218: first light at z≃5.6?
o	Fig.1: <[ESK2001] a> (Nos a-c), <[ESK2001] GN> (Nos G1-G2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ESK2003]
[ESK2003]	(Evans+Seward+Krauss+, 2003)
Write:	<<[ESK2003] NNN>> <<[ESK2003] NotDetected NN>>
N:	154+23
Object:	* (SIMBAD class: Star)
Note:	Chandra observations. Tables 1, 2: X-ray sources identified or not as OB stars in the field of eta Car. Table 7: not detected OB stars. See also 2001ApJ...553..832S. See also [ESW2004].
Ref:	=2003ApJ...589..509E
by	EVANS N.R. , SEWARD F.D., KRAUSS M.I., ISOBE T., NICHOLS J., SCHLEGEL E.M., WOLK S.J.
	Astrophys. J., 589, 509-525 (2003)
	Chandra observations of associates of η Carinae. I. Luminosities.
o	Tables 1, 2: <[ESK2003] NNN> N=154 among (Nos 1-167). Table 7: <[ESK2003] NotDetected NN> N=23 among (Nos 1-32).
=E=	Catalogue in electronic form as J/ApJ/589/509
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ESM2009]
[ESM2009]
Write:	<<[ESM2009] NNN>>
N:	427
Object:	* (SIMBAD class: Star)
Note:	VLT NACO AO-assisted NIR observations of the Arches cluster.
in source:	NAME Arches Cluster
Ref:	=2009A&A...501..563E
by	ESPINOZA P. , SELMAN F.J., MELNICK J.
	Astron. Astrophys., 501, 563-583 (2009)
	The massive star initial mass function of the Arches cluster.
o	Table 2: <[ESM2009] NNN> (Nos 1-427).
=E=	Catalogue in electronic form as J/A+A/501/563
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ESM2017]
[ESM2017]	(Ellison+Secrest+Mendel+, 2017)
Write:	<<[ESM2017] XN>>
N:	2
Object:	AGN (SIMBAD class: AGN = Active Galaxy Nucleus)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-S observations of N=2 X-ray sources, a dual AGN in SDSS J140737.17+442856.2.
in source:	SDSS J140737.17+442856.2
Ref:	=2017MNRAS.470L..49E
by	ELLISON S.L. , SECREST N.J., MENDEL J.T., SATYAPAL S., SIMARD L.
	Mon. Not. R. Astron. Soc., 470L, 49-53 (2017)
	Discovery of a dual active galactic nucleus with ~8 kpc separation.
o	Fig. 2, Table 1: <[ESM2017] XN> (Nos X1-X2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ESO
ESO	(European Southern Obs.) (Not yet in Simbad)
Write:	<<ESO HHMMSS+DDMM.m>>
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	687 objects from 'ESO' catalogues are compiled as PN
Ref:	=1982ESO...C......0L
by	LAUBERTS A.
	The ESO/Uppsala Survey of the ESO(B) Atlas, 0-503 (1982)
	The ESO/Uppsala Survey of the ESO(B) Atlas.
o	<ESO FFF-NNN> N=18438.
Details on Acronym: ESO
ESO	(European Southern Obs.)
Write:	<<ESO FFF-NNN>> <<ESO FFFANNN>> (not recognised by Simbad, but found in literature) <<ESO FFFAANNN>> <<ESO FFF-ANNN>> <<ESO FFF-AANNN>>
N:	18438
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat.	in SIMBAD: for G only
Note:	Discovery name. Format 'FFF-TTT NN' is the original format: 'TTT' is the type, it is an information, not an identifier. This format is not used in SIMBAD. 687 objects from catalogues are compiled as PN. Revised and superseded by Lauberts, 1982.
Ref:	=1974A&AS...18..463H
by	HOLMBERG E.B. , LAUBERTS A., SCHUSTER H.E., WEST R.M.
	Astron. Astrophys., Suppl. Ser., 18, 463-489 (1974)
	The ESO/Uppsala survey of the ESO (B) atlas of south sky 1.
o	20 fields.
o	<ESO FFF-NN> N=420
Ref:	=1974A&AS...18..491H
by	HOLMBERG E.B. , LAUBERTS A., SCHUSTER H.E., WEST R.M.
	Astron. Astrophys., Suppl. Ser., 18, 491-509 (1974)
	The ESO/Uppsala survey of the ESO (B) atlas of southern sky. II.
o	16 fields.
o	<ESO FFF-NN> N=446
Ref:	=1975A&AS...22..327H
by	HOLMBERG E.B. , LAUBERTS A., SCHUSTER H.E., WEST R.M.
	Astron. Astrophys., Suppl. Ser., 22, 327-402 (1975)
	The ESO/Uppsala survey of the ESO (B) atlas of the southern sky. III.
o	80 fields, about 80/100 objects are new.
o	<ESO FFF-NN> N=2280
Ref:	=1977A&AS...27..295H
by	HOLMBERG E.B. , LAUBERTS A., SCHUSTER H.E., WEST R.M.
	Astron. Astrophys., Suppl. Ser., 27, 295-342 (1977)
	The ESO/Uppsala survey of the ESO (B) atlas of the southern sky. IV.
o	101 fields, about 70/100 objects are new.
o	<ESO FFF-NN> N=2920
Ref:	=1978A&AS...31...15H
by	HOLMBERG E.B. , LAUBERTS A., SCHUSTER H.E., WEST R.M.
	Astron. Astrophys., Suppl. Ser., 31, 15-54 (1978)
	The ESO/ Uppsala survey of the ESO (B) atlas of the southern sky. V.
o	78 fields, about 70/100 objects are new.
o	<ESO FFF-NN> N=2395
Ref:	=1978A&AS...34..285H
by	HOLMBERG E.B. , LAUBERTS A., SCHUSTER H.E., WEST R.M.
	Astron. Astrophys., Suppl. Ser., 34, 285-340 (1978)
	The ESO-Uppsala survey of the ESO (B) atlas of the southern sky. VI.
o	98 fields, about 90/100 objects are new.
o	<ESO FFF-NN> N=3162
Ref:	=1980A&AS...39..173H
by	HOLMBERG E.B. , LAUBERTS A., SCHUSTER H.E., WEST R.M.
	Astron. Astrophys., Suppl. Ser., 39, 173-195 (1980)
	The ESO/Uppsala survey of the ESO (b) atlas of the southern sky. VII.
o	72 fields, about 50/100 objects are new.
o	<ESO FFF-NN> N=2395
Ref:	=1981A&AS...43..307L
by	LAUBERTS A. , HOLMBERG E.B., SCHUSTER H.E., WEST R.M.
	Astron. Astrophys., Suppl. Ser., 43, 307-329 (1981)
	The ESO/Uppsala survey of the ESO (b) atlas of the southern sky - VIII.
o	78 fields, about 50/100 objects are new.
o	<ESO FFF-NN> N=2597
Ref:	=1981A&AS...46..311L
by	LAUBERTS A. , HOLMBERG E.B., SCHUSTER H.E., WEST R.M.
	Astron. Astrophys., Suppl. Ser., 46, 311-346 (1981)
	The ESO/Uppsala survey of the ESO (b) atlas of the southern sky. IX.
o	64 fields, about 50/100 objects are new.
o	<ESO FFF-NN> N=1881
Ref:	=1982ESO...C......0L
by	LAUBERTS A.
	The ESO/Uppsala Survey of the ESO(B) Atlas, 0-503 (1982)
	The ESO/Uppsala Survey of the ESO(B) Atlas.
o	<ESO FFF-NNN> N=18438.
=E=	Catalogue in electronic form as VI/30
=E=	Catalogue in electronic form as VII/34
Details on Acronym: ESO
ESO	(European Southern Obs.)
*****	Avoid the usage of ESO, prefer Ruiz
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ESO-H-alpha
ESO-H-alpha	(European Southern Obs., H-alpha)
*****	Avoid the usage of ESO-H-alpha, prefer ESO-HA
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ESO-HA
ESO-HA	(European Southern Obs., H-Alpha)= (ESO-H-alpha)
Write:	<<ESO-HA NNNNWa>>
N:	575+2+1259+2+289+64
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Note:	(Nos 1-1834) but some Nos are missing: 280, 283, 285-289. ESO-HA 279 and ESO-HA 1397 are binaries (Nos 279a-279b, 1397E-1397W).
Ref:	=1992A&A...256L...1R
by	REIPURTH B. , EIROA C.
	Astron. Astrophys., 256, 1-4 (1992)
	Discovery of four Herbig-Haro objects in Serpens.
o	<HH NNN> (Nos 106-109), <ESO-HA 279>
Ref:	=1994A&AS..104..233P
by	PETTERSSON B. , REIPURTH B.
	Astron. Astrophys., Suppl. Ser., 104, 233-258 (1994)
	Young stars associated with the Vela Molecular Ridge. I. VMR clouds C and D, Collinder 197 and Vela R2.
o	Table 2: <ESO-HA NNN> (Nos 1-278).
Ref:	=1994A&A...288..165A
by	ASPIN C. , REIPURTH B., LEHMANN T.
	Astron. Astrophys., 288, 165-174 (1994)
	Is ESO Hα 279 a pre-main sequence binary ?
o	<ESO-HA NNNa> (Nos 279a, 279b) added.
Ref:	=1995A&AS..114..135C
by	CHELLI A. , CRUZ-GONZALEZ I., REIPURTH B.
	Astron. Astrophys., Suppl. Ser., 114, 135-142 (1995)
	Near infrared observations of southern young multiple systems.
o	B 59-2 = NAME B 59-2
o	Table 1: <ESO-HA NNN> (No. 282) added.
Ref:	=1996A&AS..120..229R
by	REIPURTH B. , PEDROSA A., LAGO M.T.V.T.
	Astron. Astrophys., Suppl. Ser., 120, 229-256 (1996)
	Hα emission in pre-main sequence stars. I. An atlas of line profiles.
o	Table 1: <ESO-HA NNN> (No. 300) added.
Ref:	=1997A&A...321..220B
by	BRANDNER W. , ZINNECKER H.
	Astron. Astrophys., 321, 220-228 (1997)
	Physical properties of 90AU to 250AU pre-main-sequence binaries.
o	Table 2: <ESO-HA NNN> (No. 281) added.
Ref:	=1997A&A...327.1164R
by	REIPURTH B. , OLBERG M., GREDEL R., BOOTH R.S.
	Astron. Astrophys., 327, 1164-1176 (1997)
	Herbig-Haro flows and molecular outflows in the HH 56/57 region.
o	Table 1: <ESO-HA NNN> (No. 284) added.
Ref:	=1997A&A...327.1185R
by	REIPURTH B. , CORPORON P., OLBERG M., TENORIO-TAGLE G.
	Astron. Astrophys., 327, 1185-1193 (1997)
	Thackeray's globules in IC 2944.
o	Table 2: <ESO-HA NNN> (Nos 301-307) added.
Ref:	=2004AJ....127.1117R
by	REIPURTH B. , PETTERSSON B., ARMOND T., BALLY J., VAZ L.P.R.
	Astron. J., 127, 1117-1130 (2004)
	Hα emission-line stars in molecular clouds. I. The NGC 2264 region.
o	Table 2: <ESO-HA NNN> (Nos 308-551) added.
Ref:	=2004A&A...417..583C
by	COMERON F. , REIPURTH B., HENRY A., FERNANDEZ M.
	Astron. Astrophys., 417, 583-596 (2004)
	Extending the census at the bottom of the stellar mass function in Chamaeleon I.
o	Table 2: <ESO-HA NNN> (Nos 552-575) added.
Ref:	=2014A&A...570A..30P
by	PETTERSSON B. , ARMOND T., REIPURTH B.
	Astron. Astrophys., 570A, 30-30 (2014)
	Hα emission-line stars in molecular clouds. II. The M 42 region.
o	(Erratum) + corrigendum vol. 573, p. C2 (2015)
o	Figs 8-18: <ESO-HA NNNN> (Nos 576-1834), <ESO-HA NNNNW> (Nos 925E, 925W, 1397E, 1397W).
Ref:	=2019A&A...630A..90P
by	PETTERSSON B. , REIPURTH B.
	Astron. Astrophys., 630A, 90-90 (2019)
	Hα emission-line stars in molecular clouds. III. Canis Major.
o	Table 2: <ESO-HA NNNN> N=289+64 among (Nos 1835-2123, 2706-2769).
=E=	Catalogue in electronic form as J/A+AS/104/233
=E=	Catalogue in electronic form as J/AJ/127/1117
=E=	Catalogue in electronic form as J/A+A/570/A30
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ESO-LV
ESO-LV	(European Southern Obs., Lauberts+Valentijn)
Write:	<<ESO-LV FFF-NNNN>>
N:	15467
Object:	G (SIMBAD class: Galaxy)
Note:	In the format, the 'NNNN' number is always a 4 digits one. When in the format, the last digit is 0, ESO-LV FFF-NNN0 = ESO FFF-NNN (without the ending '0') for ex.: ESO-LV 314-0030 = ESO 314-3, ESO-LV 440-0170 = ESO 440-17
Ref:	=1989ESOLV.C......0L
by	LAUBERTS A. , VALENTIJN E.A.
	The Surface Photometry Catalogue of the ESO-Uppsala Galaxies, 0-None (1989)
	The surface photometry catalogue of the ESO-Uppsala galaxies.
o	<ESO-LV FFF-NNNN> N=15467
=E=	Catalogue in electronic form as VII/115
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ESP
ESP	(ESO Slice Project)
Write:	<<ESP NNNNN>>
N:	4487
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Galaxy redshift survey in a region near the SGP: format 'NNNNN', always a 5 digits format. See also [RZZ99], ESP groups of galaxies.
Ref:	=1998A&AS..130..323V
by	VETTOLANI G. , ZUCCA E., MERIGHI R., MIGNOLI M., PROUST D., ZAMORANI G., CAPPI A., GUZZO L., MACCAGNI D., RAMELLA M., STIRPE G.M., BLANCHARD A., CAYATTE V., COLLINS C., MacGILLIVRAY H., MAUROGORDATO S., SCARAMELLA R., BALKOWSKI C., CHINCARINI G., FELENBOK P.
	Astron. Astrophys., Suppl. Ser., 130, 323-332 (1998)
	The ESO Slice Project (ESP) galaxy redshift survey. III. The sample.
o	<ESP NNNNN> N=4487 among N>40477
=E=	Catalogue in electronic form as J/A+AS/130/323
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ESP
ESP	(ESO Slice Project)
*****	Avoid the usage of ESP, prefer [RZZ99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ESR2018]
[ESR2018]	(Ebeling+Stockmann+Richard+, 2018)
Write:	<<[ESR2018] eMACSJ1341-QG-1>> <<[ESR2018] eMACS J1341.9-2442 m1.N>>
N:	1+3
Object:	G + Grav. lensed image of a G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST WFC3 and VLT X-SHOOTER observations of N=1 quiescent background galaxy and its N=3 lensed images.
Ref:	=2018ApJ...852L...7E
by	EBELING H. , STOCKMANN M., RICHARD J., ZABL J., BRAMMER G., TOFT S., MAN A.
	Astrophys. J., 852L, 7-7 (2018)
	Thirty-fold: extreme gravitational lensing of a quiescent galaxy at z = 1.6.
o	<eMACS JHHMM.m+DDMM> (No. J1341.9-2442) added. <[ESR2018] eMACSJ1341-QG-1> N=1. Fig. 1: <[ESR2018] eMACS J1341.9-2442 m1.N> (Nos m1.1-m1.3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ESS2003]
[ESS2003]	(Erb+Shapley+Steidel+, 2003)= ([ESS2003a])
Write:	<<[ESS2003] {Q}HHMM-{C\|D\|M}NNNN>> <<[ESS2003] QHHMM-BMNNNN>> <<[ESS2003] QHHMM-BXNNNN>> <<[ESS2003] QHHMM-MDNNNN>> <<[ESS2003] QHHMM-BNBNNN>>
Object:	G (SIMBAD class: Galaxy)
Note:	NIRSPEC Keck II observations. Search for galaxies with z>2 in several QSO fields. See also [PSL2007] and [PKS98], [PSS2001], [SAD98], [SSP2004], Westphal.
Ref:	=2003ApJ...591..101E
by	ERB D.K. , SHAPLEY A.E., STEIDEL C.C., PETTINI M., ADELBERGER K.L., HUNT M.P., MOORWOOD A.F.M., CUBY J.-G.
	Astrophys. J., 591, 101-118 (2003)
	Hα spectroscopy of galaxies at z > 2: kinematics and star formation.
o	Table 1: <[PSS2001] CDFb AANN> (No. BN88) added, <Westphal AANNN> (No. BX600) added. Table 1: <[ESS2003] QHHMM-AANNN> N=12.
Ref:	=2004ApJ...604..534S
by	STEIDEL C.C. , SHAPLEY A.E., PETTINI M., ADELBERGER K.L., ERB D.K., REDDY N.A., HUNT M.P.
	Astrophys. J., 604, 534-550 (2004)
	A survey of star-forming galaxies in the 1.4≲Z≲ 2.5 redshift desert: overview.
o	Table 4: <[ESS2003] QHHMM-AANNNN> N=6. Table 4: <[SSP2004] GWS-AANNNN>, <[SSP2004] HDF-AANNNN>, <[SSP2004] HDF-AAANNNN>, N=5.
Ref:	=2004ApJ...612..108S
by	SHAPLEY A.E. , ERB D.K., PETTINI M., STEIDEL C.C., ADELBERGER K.L.
	Astrophys. J., 612, 108-121 (2004)
	Evidence for solar metallicities in massive star-forming galaxies at z ≳ 2.
o	Table 1: <[ESS2003] Q1623-AANNN> N=8 added.
Ref:	=2005ApJ...626..698S
by	SHAPLEY A.E. , STEIDEL C.C., ERB D.K., REDDY N.A., ADELBERGER K.L., PETTINI M., BARMBY P., HUANG J.
	Astrophys. J., 626, 698-722 (2005)
	Ultraviolet to mid-infrared observations of star-forming galaxies at z~2: stellar masses and stellar populations.
o	Table 2: <[ESS2003] Q1700-BXNNNN>, <[ESS2003] Q1700-MDNNNN>, N=69 new.
Ref:	=2005ApJ...629..636A
by	ADELBERGER K.L. , SHAPLEY A.E., STEIDEL C.C., PETTINI M., ERB D.K., REDDY N.A.
	Astrophys. J., 629, 636-653 (2005)
	The connection between galaxies and intergalactic absorption lines at redshift 2≲z≲3.
o	Table 2: <[ESS2003] Q1623-BXNNN> N=2 added, <[ESS2003] Q2343-BXNNN> N=1 added. Table 3: <[ESS2003] Q2346-BXNNN> N=2 added.
o	Table 2: Q2342+125 is not identified, Q2343+125 = [HB93] 2343+125, Q2344+125 = [HB93] 2344+125.
Ref:	=2006ApJ...637..648S
by	SIMCOE R.A. , SARGENT W.L.W., RAUCH M., BECKER G.
	Astrophys. J., 637, 648-668 (2006)
	Observations of chemically enriched QSO absorbers near z~2.3 galaxies: galaxy formation feedback signatures in the intergalactic medium.
o	Table 1: <[ESS2003] Q1700-BXNNN>, <[ESS2003] Q1700-MDNN>, N=6 added.
Ref:	=2006ApJ...645.1062F
by	FORSTER SCHREIBER N.M. , GENZEL R., LEHNERT M.D., BOUCHE N., VERMA A., ERB D.K., SHAPLEY A.E., STEIDEL C.C., DAVIES R., LUTZ D., NESVADBA N., TACCONI L.J., EISENHAUER F., ABUTER R., GILBERT A., GILLESSEN S., STERNBERG A.
	Astrophys. J., 645, 1062-1075 (2006)
	SINFONI integral field spectroscopy of z ~ 2 UV-selected galaxies: rotation curves and dynamical evolution.
o	Table 1: <[ESS2003] Q1623BXNNN> N=4 added, <[ESS2003] Q2343-BXNNN> N=4 added.
Ref:	=2006ApJ...646..107E
by	ERB D.K. , STEIDEL C.C., SHAPLEY A.E., PETTINI M., REDDY N.A., ADELBERGER K.L.
	Astrophys. J., 646, 107-132 (2006)
	The stellar, gas, and dynamical masses of star-forming galaxies at z ~ 2.
o	Table 1: <[ESS2003] Q1623-AANNN>, <[ESS2003] Q1700-AANNN>, N=15 added, <[ESS2003] Q2343-AANNN> N=22 added. Table 1: <[SSP2004] HDF-AANNNN>, [SSP2004] HDF-AAANNNN> N=20 added. Table 1: <Westphal AANNN> N=1 added.
Ref:	=2007ApJ...668...23P
by	PETER A.H.G. , SHAPLEY A.E., LAW D.R., STEIDEL C.C., ERB D.K., REDDY N.A., PETTINI M.
	Astrophys. J., 668, 23-44 (2007)
	Morphologies of galaxies in and around a protocluster at z = 2.300.
o	Figs 2-4: <[ESS2003] Q1700-BXNNNN> N=22 added, <[ESS2003] Q1700-MDNNNN> N=14 added. Figs 2-4: <[PSL2007] Q1700-ANN> N=9, Fig.5: <[PSL2007] Q1700-DRGNN> N=43 among (Nos 17-75).
Ref:	=2007ApJ...669..929L
by	LAW D.R. , STEIDEL C.C., ERB D.K., LARKIN J.E., PETTINI M., SHAPLEY A.E., WRIGHT S.A.
	Astrophys. J., 669, 929-946 (2007)
	Integral field spectroscopy of high-redshift star-forming galaxies with laser-guided adaptive optics: evidence for dispersion-dominated kinematics.
o	Table 1: <[ESS2003] Q0449-BXNN> (No. BX93) added.
Ref:	=2007ApJ...670...15R
by	RIX S.A. , PETTINI M., STEIDEL C.C., REDDY N.A., ADELBERGER K.L., ERB D.K., SHAPLEY A.E.
	Astrophys. J., 670, 15-38 (2007)
	The sightline to Q2343-BX415: clues to galaxy formation in a quasar environment.
o	Table 8: <[RPS2007] QSO J2346+1247 abs N.NNNN> N=11 = <[RPS2007] SNN> (Nos S1-S11). Table 8, Fig.14: <[ESS2003] Q2343-DNN> (Nos D25, D29), <[ESS2003] Q2343-BXNNN> (Nos BX333, BX417, BX484) added.
o	Fig.14: Objects [ESS2003] Q2343-AANNN are not in SIMBAD.
Ref:	=2008ApJ...676..816G
by	GONCALVES T.S. , STEIDEL C.C., PETTINI M.
	Astrophys. J., 676, 816-835 (2008)
	Detection of the transverse proximity effect: radiative feedback from bright QSOs.
o	Table 5, Fig.17: <[ESS2003] Q1623-BXNNN>, <[ESS2003] Q1623-MDNNN>, N=10 added.
Ref:	=2012ApJ...745...33K
by	KULAS K.R. , SHAPLEY A.E., KOLLMEIER J.A., ZHENG Z., STEIDEL C.C., HAINLINE K.N.
	Astrophys. J., 745, 33 (2012)
	The kinematics of multiple-peaked Lyα emission in star-forming galaxies at z ~ 2-3.
o	Table 1: <[ESS2003] QHHMM-AANNN>, N=12 added.
Ref:	=2014ApJ...795...33E
by	ERB D.K. , STEIDEL C.C., TRAINOR R.F., BOGOSAVLJEVIC M., SHAPLEY A.E., NESTOR D.B., KULAS K.R., LAW D.R., STROM A.L., RUDIE G.C., REDDY N.A., PETTINI M., KONIDARIS N.P., MACE G., MATTHEWS K., McLEAN I.S.
	Astrophys. J., 795, 33 (2014)
	The Lyα properties of faint galaxies at z ~ 2-3 with systemic redshifts and velocity dispersions from Keck-MOSFIRE.
o	Table 1: <[ESS2003] Q1700-BNBNNN> N=17 among (Nos 17-157).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ESS2003a]
[ESS2003a]	(Erb+Shapley+Steidel+, 2003)
*****	Avoid the usage of [ESS2003a], prefer [ESS2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ESS2003b]
[ESS2003b]	(Edge+Smith+Sand+, 2003)
Write:	<<[ESS2003b] ANa>> <<[ESS2003b] Galaxy>>
N:	2+6+1
Object:	Grav. lensed image + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST image of ACO 1201. A gravitational arc A1 is observed, with a faint feature A2, arising from the gravitational distortion of a background galaxy by the cluster.
Ref:	=2003ApJ...599L..69E
by	EDGE A.C. , SMITH G.P., SAND D.J., TREU T., EBELING H., ALLEN S.W., VAN DOKKUM P.G.
	Astrophys. J., 599, 69-72 (2003)
	A unique small-scale gravitational arc in A1201.
o	<[ESS2003b] ANa> (Nos A1-A2, A1a-A1f), <[ESS2003b] Galaxy> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ESS2004]
[ESS2004]	(Erb+Steidel+Shapley+, 2004)
Write:	<<[ESS2004] GOODS-N BXNNNN>>
N:	13
Object:	G (SIMBAD class: Galaxy)
Note:	KeckII NIR observations of 13 galaxies at z 2 in the GOODS North field.
in source:	NAME GOODS North Field
Ref:	=2004ApJ...612..122E
by	ERB D.K. , STEIDEL C.C., SHAPLEY A.E., PETTINI M., ADELBERGER K.L.
	Astrophys. J., 612, 122-130 (2004)
	The kinematics of morphologically selected z~2 galaxies in the GOODS-North field.
o	Table 1: <[ESS2004] GOODS-N BXNNNN> N=13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ESS2013]
[ESS2013]	(Eichner+Seitz+Suyu+, 2013)
Write:	<<[ESS2013] NNa.N>>
N:	52
Object:	Grav. lensed image of a G (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy)
Note:	N=52 images of 13 background galaxies lensed by the cluster MCS J1206.2-0847. Use of HST CLASH data.
in source:	MCS J1206.2-0847
Ref:	=2013ApJ...774..124E
by	EICHNER T. , SEITZ S., SUYU S.H., HALKOLA A., UMETSU K., ZITRIN A., COE D., MONNA A., ROSATI P., GRILLO C., BALESTRA I., POSTMAN M., KOEKEMOER A., ZHENG W., HOST O., LEMZE D., BROADHURST T., MOUSTAKAS L., BRADLEY L., MOLINO A., NONINO M., MERCURIO A., SCODEGGIO M., BARTELMANN M., BENITEZ N., BOUWENS R., DONAHUE M., INFANTE L., JOUVEL S., KELSON D., LAHAV O., MEDEZINSKI E., MELCHIOR P., MERTEN J., RIESS A.
	Astrophys. J., 774, 124 (2013)
	Galaxy halo truncation and giant arc surface brightness reconstruction in the cluster MACSJ1206.2-0847.
o	Fig. 3, Table 2: <[ESS2013] NNa.N> N=52.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ESS2017]
[ESS2017]	(Ergin+Sezer+Sano+, 2017)
Write:	<<[ESS2017] PS JHHMM.m+DDMM>>
N:	2
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	N=2 gamma-ray sources in the field of the supernova remnant 3C 400.2, in archival Fermi-LAT observations.
in source:	3C 400.2
Ref:	=2017ApJ...842...22E
by	ERGIN T. , SEZER A., SANO H., YAMAZAKI R., FUKUI Y.
	Astrophys. J., 842, 22-22 (2017)
	Recombining plasma and γ-ray emission in the mixed-morphology supernova remnant 3C 400.2.
o	<[ESS2017] PS JHHMM.m+DDMM> (Nos PS J1934.5+1845, PS J1938.6+1722).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ESSENCE
ESSENCE	(Equation of State, SuperNovae trace Cosmic Expansion)= (SN)
Write:	<<ESSENCE aNNN>>
N:	138
Object:	SN (SIMBAD class: Supernova = SuperNova)
Stat:	is completely incorporated in Simbad
Note:	ESSENCE supernovae survey.
Ref:	=2007ApJ...666..674M
by	MIKNAITIS G. , PIGNATA G., REST A., WOOD-VASEY W.M., BLONDIN S., CHALLIS P., SMITH R.C., STUBBS C.W., SUNTZEFF N.B., FOLEY R.J., MATHESON T., TONRY J.L., AGUILERA C., BLACKMAN J.W., BECKER A.C., CLOCCHIATTI A., COVARRUBIAS R., DAVIS T.M., FILIPPENKO A.V., GARG A., GARNAVICH P.M., HICKEN M., JHA S., KRISCIUNAS K., KIRSHNER R.P., LEIBUNDGUT B., LI W., MICELI A., NARAYAN G., PRIETO J.L., RIESS A.G., SALVO M.E., SCHMIDT B.P., SOLLERMAN J., SPYROMILIO J., ZENTENO A.
	Astrophys. J., 666, 674-693 (2007)
	The ESSENCE supernova survey: survey optimization, observations, and supernova photometry.
o	Table 3, col(1): when several lines have the same SN YYYYaa designation, only the first line is the real SN YYYYaa, to cross-identify with the ESSENCE aNNN on the same line. On the other lines, objects are only ESSENCE aNNN objects.
o	Table 3, col(4): <ESSENCE aNNN> N=138.
Ref:	=2016ApJS..224....3N
by	NARAYAN G. , REST A., TUCKER B.E., FOLEY R.J., WOOD-VASEY W.M., CHALLIS P., STUBBS C., KIRSHNER R.P., AGUILERA C., BECKER A.C., BLONDIN S., CLOCCHIATTI A., COVARRUBIAS R., DAMKE G., DAVIS T.M., FILIPPENKO A.V., GANESHALINGAM M., GARG A., GARNAVICH P.M., HICKEN M., JHA S.W., KRISCIUNAS K., LEIBUNDGUT B., LI W., MATHESON T., MIKNAITIS G., PIGNATA G., PRIETO J.L., RIESS A.G., SCHMIDT B.P., SILVERMAN J.M., SMITH R.C., SOLLERMAN J., SPYROMILIO J., SUNTZEFF N.B., TONRY J.L., ZENTENO A.
	Astrophys. J., Suppl. Ser., 224, 3 (2016)
	Light curves of 213 type Ia supernovae from the ESSENCE survey.
o	Table 6: <ESSENCE aNNN> N=213.
=E=	Catalogue in electronic form as J/ApJ/666/674
=E=	Catalogue in electronic form as <J/ApJS/224/3/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ESW2004]
[ESW2004]	(Evans+Schlegel+Waldron+, 2004)
Write:	<<[ESW2004] A>>
N:	16
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra image of the field of eta Car. All objects already have a [ESK2003] NNN name from Paper I.
Ref:	=2004ApJ...612.1065E
by	EVANS N.R. , SCHLEGEL E.M., WALDRON W.L., SEWARD F.D., KRAUSS M.I., NICHOLS J., WOLK S.J.
	Astrophys. J., 612, 1065-1080 (2004)
	Chandra observations of associates of η Carinae. II. Spectra.
o	Table 1: <[ESW2004] A> (Nos A-P).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ET
ET	(Einasto+Tago+)
*****	Avoid the usage of ET, prefer SCl
Origin	of the Acronym: L (1998ApJ...506..509K)
Details on Acronym: ET
ET	(Elephant Trunk)
*****	Avoid the usage of ET, prefer [SHB80]
Origin	of the Acronym: L (2003AJ....126.1423K)
Details on Acronym: [ETC2005]
[ETC2005]	(Eiroa+Torrelles+Curiel+, 2005)= (VLA)
Write:	<<[ETC2005] NN>> <<[ETC2005] NN'>>
N:	20+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 3.5cm continuum observations of the Serpens Cloud core.
in source:	NAME Serpens Cloud
Ref:	=2005AJ....130..643E
by	EIROA C. , TORRELLES J.M., CURIEL S., DJUPVIK A.A.
	Astron. J., 130, 643-651 (2005)
	Very large array 3.5 cm continuum sources in the Serpens cloud core.
o	Table 2: <[ETC2005] NN> (Nos 1-20), <[ETC2005] NN'> (No. 19').
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ETM94]
[ETM94]	(Eiroa+Torrelles+Miranda+, 1994)
Write:	<<[ETM94] AFGL 5142 Star N>> <<[ETM94] CB 39 Star N>> <<[ETM94] IRAS 22376+7455 Star N>> <<[ETM94] IRAS 22376+7455 RN>>
N:	1+1+3+1
Object:	* + RN (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 3, Fig.3: N=1 star in the field of AFGL 5142. Table 3: N=1 star in the field of [CB88] 39. Table 3, Fig.5: N=3 stars in the field of IRAS 22376+7455. Fig.5: N=1 reflexion nebula in the field of IRAS 22376+7455.
Ref:	=1994A&AS..108...73E
by	EIROA C. , TORRELLES J.M., MIRANDA L.F., ANGLADA G., ESTALELLA R.
	Astron. Astrophys., Suppl. Ser., 108, 73-78 (1994)
	Optical nebulosities associated with IRAS sources in dense cloud cores.
o	Table 3: <[ETM94] AFGL 5142 Star N> (No. 1), <[ETM94] CB 39 Star N> (No. 1), <[ETM94] IRAS 22376+7455 Star N> (Nos 1-3). Fig.5: <[ETM94] IRAS 22376+7455 RN> (No. R1). Table 3: <HH NNNA> (Nos 189, 190).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ETP2005]
[ETP2005]	(Ebisawa+Tsujimoto+Paizis+, 2006)
Write:	<<[ETP2005] X NNN>> <<[ETP2005] NIR NNNNN>>
N:	274+32398
Object:	(X) + (Near IR) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	New X-ray sources detected with Chandra (see CXOGPE) in the galactic plane. Complementary NIR survey with SofI at ESO/NTT for source identification.
Ref:	=2005ApJ...635..214E
by	EBISAWA K. , TSUJIMOTO M., PAIZIS A., HAMAGUCHI K., BAMBA A., CUTRI R., KANEDA H., MAEDA Y., SATO G., SENDA A., UENO M., YAMAUCHI S., BECKMANN V., COURVOISIER T.J.-L., DUBATH P., NISHIHARA E.
	Astrophys. J., 635, 214-242 (2005)
	Chandra deep X-ray observation of a typical Galactic plane region and near-infrared identification.
o	Fig. 12 : CXOU J184357-035441 (incomplete format) = EQ J184357-035441 in SIMBAD
o	Table 1: <CXOGPE JHHMMSS.s+DDMMSS> N=274 = <[ETP2005] X NNN> (Nos 1-274). Table 2: <[ETP2005] NIR NNNNN> (Nos 1-32398).
=E=	Catalogue in electronic form as J/ApJ/635/214
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EUC2020
EUC2020	(Euclid Collaboration, 2020)
Write:	<<EUC2020 NNNNNN>>
N:	413
Object:	G (SIMBAD class: Galaxy)
Note:	VLT KMOS observations of N=413 galaxies, as part of the Complete Calibration of the Color–Redshift Relation (C3R2) survey. See also [MSC2017], [MSC2019], and [SMD2021].
Ref:	=2020A&A...642A.192E
by	EUCLID COLLABORATION , GUGLIELMO V., SAGLIA R., CASTANDER F.J., GALAMETZ A., PALTANI S., BENDER R., BOLZONELLA M., CAPAK P., ILBERT O., MASTERS D.C., STERN D., ANDREON S., AURICCHIO N., BALAGUERA-ANTOLINEZ A., BALDI M., BARDELLI S., BIVIANO A., BODENDORF C., BONINO D., BOZZO E., BRANCHINI E., BRAU-NOGUE S., BRESCIA M., BURIGANA C., CABANAC R.A., CAMERA S., CAPOBIANCO V., CAPPI A., CARBONE C., CARRETERO J., CARVALHO C.S., CASAS R., CASAS S., CASTELLANO M., CASTIGNANI G., CAVUOTI S., CIMATTI A., CLEDASSOU R., COLODRO-CONDE C., CONGEDO G., CONSELICE C.J., CONVERSI L., COPIN Y., CORCIONE L., COSTILLE A., COUPON J., COURTOIS H.M., CROPPER M., DA SILVA A., DE LA TORRE S., DI FERDINANDO D., DUBATH F., DUNCAN C.A.J., DUPAC X., DUSINI S., FABRICIUS M., FARRENS S., FERREIRA P.G., FOTOPOULOU S., FRAILIS M., FRANCESCHI E., FUMANA M., GALEOTTA S., GARILLI B., GILLIS B., GIOCOLI C., GOZALIASL G., GRACIA-CARPIO J., GRUPP F., GUZZO L., HILDEBRANDT H., HOEKSTRA H., HORMUTH F., ISRAEL H., JAHNKE K., KEIHANEN E., KERMICHE S., KILBINGER M., KIRKPATRICK C.C., KITCHING T., KUBIK B., KUNZ M., KURKI-SUONIO H., LAUREIJS R., LIGORI S., LILJE P.B., LLORO I., MAINO D., MAIORANO E., MARASTON C., MARGGRAF O., MARTINET N., MARULLI F., MASSEY R., MAUROGORDATO S., MEDINACELI E., MEI S., MENEGHETTI M., METCALF R.B., MEYLAN G., MORESCO M., MOSCARDINI L., MUNARI E., NAKAJIMA R., NEISSNER C., NIEMI S., NUCITA A.A., PADILLA C., PASIAN F., PATRIZII L., POCINO A., PONCET M., POZZETTI L., RAISON F., RENZI A., RHODES J., RICCIO G., ROMELLI E., RONCARELLI M., ROSSETTI E., SANCHEZ A.G., SAPONE D., SCHNEIDER P., SCOTTEZ V., SECROUN A., SERRANO S., SIRIGNANO C., SIRRI G., SUREAU F., TALLADA-CRESPI P., TAVAGNACCO D., TAYLOR A.N., TENTI M., TERENO I., TOLEDO-MOREO R., TORRADEFLOT F., TRAMACERE A., VALENZIANO L., VASSALLO T., WANG Y., WELIKALA N., WETZSTEIN M., WHITTAKER L., ZACCHEI A., ZAMORANI G., ZOUBIAN J., ZUCCA E.
	Astron. Astrophys., 642A, 192-192 (2020)
	Euclid preparation. VIII. The Complete Calibration of the Colour-Redshift Relation survey: VLT/KMOS observations and data release.
o	<EUC2020 NNNNNN> N=413 among (Nos 27970-824725).
=E=	Catalogue in electronic form as <J/A+A/642/A192/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EUVE
EUVE	(Extreme UltraViolet Explorer)
Write:	<<EUVE JHHMM+DD.d>>
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Note:	Systematic Designation
Ref:	=1994AJ....107..751M
by	MALINA R.F. , MARSHALL H.L., ANTIA B., CHRISTIAN C.A., DOBSON C.A., FINLEY D.S., FRUSCIONE A., GIROUARD F.R., HAWKINS I., JELINSKY P., LEWIS J.W., McDONALD J.S., McDONALD K., PATTERER R.J., SABA V.W., SIRK M., STROOZAS B.A., VALLERGA J.V., VEDDER P.W., WIERCIGROCH A., BOWYER S.
	Astron. J., 107, 751-764 (1994)
	Extreme ultraviolet Explorer bright source list.
o	(from ApJ/AJ CD-ROM Series, vol. 2, 1994)
o	<EUVE JHHMM+DD.d> N=356
Ref:	=1994ApJS...93..569B
by	BOWYER S. , LIEU R., LAMPTON M., LEWIS J., WU X., DRAKE J.J., MALINA R.F.
	Astrophys. J., Suppl. Ser., 93, 569-587 (1994)
	The first Extreme Ultraviolet Explorer source catalog.
o	<EUVE JHHMM+DD.d> N=410
Ref:	=1996ApJS..102..129B
by	BOWYER S. , LAMPTON M., LEWIS J., WU X., JELINSKY P., MALINA R.F.
	Astrophys. J., Suppl. Ser., 102, 129-160 (1996)
	The second Extreme Ultraviolet Explorer source catalog.
o	<2EUVE JHHMM+DD.d> N=734, = <EUVE JHHMM+DD.d>
Ref:	=1997ApJS..108..545L
by	LAMPTON M. , LIEU R., SCHMITT J.H.M.M., BOWYER S., VOGES W., LEWIS J., WU X.
	Astrophys. J., Suppl. Ser., 108, 545-None (1997)
	An all-sky catalog of faint extreme ultraviolet sources.
o	<EUVE JHHMM+DD.d> N=534
=E=	Catalogue in electronic form as J/AJ/107/751
=E=	Catalogue in electronic form as J/ApJS/93/569
=E=	Catalogue in electronic form as IX/35
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 2EUVE
2EUVE	(Extreme UltraViolet Explorer)
Write:	<<2EUVE JHHMM+DD.d>>
N:	734
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Ref:	=1996ApJS..102..129B
by	BOWYER S. , LAMPTON M., LEWIS J., WU X., JELINSKY P., MALINA R.F.
	Astrophys. J., Suppl. Ser., 102, 129-160 (1996)
	The second Extreme Ultraviolet Explorer source catalog.
o	<2EUVE JHHMM+DD.d> N=734, = <EUVE JHHMM+DD.d>
=E=	Catalogue in electronic form as IX/35
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EV*
EV*	(Extragalactic Variable *)= (GCVS)
Write:	<<EV* LMC VNNNN>> <<EV* SMC VNNNN>> <<EV* WLM VNNNN>> <<EV* ANNNNN VNNNN>> <<EV* SclG VNNNN>> <<EV* RetS VNNNN>> <<EV* SexA VNNNN>> <<EV* SexB VNNNN>> <<EV* LeoA VNNNN>> <<EV* LeoI VNNNN>> <<EV* HolII VNNNN>> <<EV* EFFF-NNN VNNNN>> <<EV* W-L-M VNNNN>> (not recognised by Simbad, but found in literature)
N:	10979
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	The catalogue II/205, Artyukhina+ (1996), superseded by the catalogue II/214, added extragalactic variable stars in 35 galaxies to the GCVS catalogue. See also V*.
Notes:	N=4801 in LMC, N=2398 in SMC, N=1200 in M 31, N=604 in Scl Galaxy, N=537 in M 33, N=265 in UGC 10822, N=176 in NGC 0185, N=172 in PGC 19441, N=97 in UGC 09749, N=83 in ESO 356-4, N=70 in NGC 2403, N=60 in IC 1613, N=56 in NGC 3109, N=55 in NGC 0205, N=49 in NGC 0147, N=43 in NGC 1466, N=42 in WLM, N=40 in NGC 6822, N=38 in Reticulum System, N=34 in UGC 12613, N=34 in NGC 0300, N=23 in Leo I, N=19 in NGC 5457, N=18 in NGC 5128, N=13 in Sex B, N=12 in Sex A, N=10 in Holmberg II, N=9 in NGC 4472, N=7 in NGC 3031, N=4 in Leo A, N=3 in NGC 4486, N=3 in IC 5152, N=2 in NGC 1313, N=1 in NGC 4365, N=1 in NGC 2366.
in source:	Magellanic Clouds:LMC = LMC
in source:	Magellanic Clouds:SMC = SMC
in source:	M 31
in source:	NAME Scl Galaxy
in source:	M 33
in source:	UGC 10822
in source:	NGC 185
in source:	LEDA 19441
in source:	UGC 9749
in source:	ESO 356-4
in source:	NGC 2403
in source:	IC 1613
in source:	NGC 3109
in source:	NGC 205
in source:	NGC 147
in source:	NGC 1466
in source:	NAME WLM
in source:	NGC 6822
in source:	NAME Reticulum System
in source:	UGC 12613
in source:	NGC 300
in source:	Leo I = UGC 5470
in source:	NGC 5457
in source:	NGC 5128
in source:	NAME Sextans B
in source:	NAME Sextans A
in source:	Holmberg II = DDO 50
in source:	NGC 4472
in source:	NGC 3031
in source:	NAME Leo A
in source:	NGC 4486
in source:	IC 5152
in source:	NGC 1313
in source:	NGC 4365
in source:	NGC 2366
Ref:	=2004yCat.2250....0S
by	SAMUS N.N. , DURLEVICH O.V.
	CDS/ADC Collection of Electronic Catalogues, -1-None (2004)
	Combined General Catalogue of Variable Stars.
o	Catalogue: <EV* LMC VNNNN>, <EV* SMC VNNNN>, <EV* WLM VNNNN>, <EV* MNN VNNNN>, <EV* ANNNN VNNNN> (letter A stands for N), <EV* INNNN VNNNN>, <EV* UNNNNN VNNNN>, <EV* PNNNNN VNNNN>, <EV* SclG VNNNN>, <EV* RetS VNNNN>,<EV* SexA VNNNN>, <EV* SexB VNNNN>, <EV* LeoA VNNNN>, <EV* LeoI VNNNN>, <EV* HolII VNNNN>, <EV* EFFF-NNN VNNNN>, N=10979.
=E=	Catalogue in electronic form as B/gcvs
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EVCC
EVCC	(Extended Virgo Cluster Catalog)
Write:	<<EVCC NNNN>>
N:	1589
Object:	G (SIMBAD class: Galaxy)
Note:	Catalog of galaxies in a wide region of the Virgo cluster, based on the Sloan Digital Sky Survey (SDSS) Data Release 7. The Extended Virgo Cluster Catalog (EVCC) covers an area of 725 deg^2 or 60.1 Mpc^2.
Ref:	=2014ApJS..215...22K
by	KIM S. , REY S.-C., JERJEN H., LISKER T., SUNG E.-C., LEE Y., CHUNG J., PAK M., YI W., LEE W.
	Astrophys. J., Suppl. Ser., 215, 22 (2014)
	The Extended Virgo Cluster Catalog.
o	Table 2: <EVCC NNNN> N=1589 among (Nos 1-2264).
=E=	Catalogue in electronic form as <J/ApJS/215/22/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Event
Event	(Type of obj.)
*****	Avoid the usage of Event, prefer MACHO
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [EVF2019]
[EVF2019]	(Emsellem+van der Burg+Fensch+, 2019)
Write:	<<[EVF2019] PNN>>
N:	3
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	VLT MUSE observations of N=3 planetary nebulae (PN) in the ultra-diffuse galaxy [VDC2018] NGC1052-DF2.
in source:	[KKS2000] 4 = [VDC2018] NGC1052-DF2
Ref:	=2019A&A...625A..76E
by	EMSELLEM E. , VAN DER BURG R.F.J., FENSCH J., JERABKOVA T., ZANELLA A., AGNELLO A., HILKER M., MULLER O., REJKUBA M., DUC P.-A., DURRELL P., HABAS R., LELLI F., LIM S., MARLEAU F.R., PENG E., SANCHEZ-JANSSEN R.
	Astron. Astrophys., 625A, 76-76 (2019)
	The ultra-diffuse galaxy NGC 1052-DF2 with MUSE. I. Kinematics of the stellar body.
o	Fig. 1, Table 1: <[EVF2019] PNN> (Nos PN1-PN3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EVM2000]
[EVM2000]	(Erben+Van Waerbeke+Mellier+, 2000) (Not yet in Simbad)
Write:	<<[EVM2000] A>>
N:	3
Object:	Clump (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 1, Fig.10: N=3 dark clumps near ACO 1942, Clump A = ACO 1942.
Ref:	=2000A&A...355...23E
by	ERBEN T. , VAN WAERBEKE L., MELLIER Y., SCHNEIDER P., CUILLANDRE J.-C., CASTANDER F.J., DANTEL-FORT M.
	Astron. Astrophys., 355, 23-36 (2000)
	Mass-detection of a matter concentration projected near the cluster Abell 1942: Dark clump or high-redshift cluster?
o	Table 1, Fig.10: <[EVM2000] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EVM96]
[EVM96]	(Ellingsen+Von Bibra+McCulloch+, 1996)
Write:	<<[EVM96] LLL.ll+B.bb>>
N:	50
Object:	CH3OH Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	See also [E2005].
Ref:	=1996MNRAS.280..378E
by	ELLINGSEN S.P. , VON BIBRA M.L., McCULLOCH P.M., NORRIS R.P., DESHPANDE A.A., PHILLIPS C.J.
	Mon. Not. R. Astron. Soc., 280, 378-396 (1996)
	A survey of the Galactic plane for 6.7-GHz methanol masers. I. l = 325°.-335°.; b = -0.53°.-0.53°.
o	Table 1: <[EVM96] LLL.ll+B.bb> N=50
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EVN2012]
[EVN2012]	(Einasto M.+Vennik J.+Nurmi+, 2014)
Write:	<<[EVN2012] NNNNN>>
N:	110
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	N=110 galaxy clusters from the SDSS DR8.
Ref:	=2012A&A...540A.123E
by	EINASTO M. , VENNIK J., NURMI P., TEMPEL E., AHVENSALMI A., TAGO E., LIIVAMAEGI L.J., SAAR E., HEINAEMAEKI P., EINASTO J., MARTINEZ V.J.
	Astron. Astrophys., 540A, 123-123 (2012)
	Multimodality in galaxy clusters from SDSS DR8: substructure and velocity distribution.
o	Table 3: <[EVN2012] NNNNN> N=110 among (Nos 18-74783).
=E=	Catalogue in electronic form as J/A+A/540/A123
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EVR
EVR	(Evryscope)
Write:	<<EVR JHHMMSS.ss+DDMMSS.s>> <<EVR -CB-NNN>> <<EVR -HSD-NNN>>
N:	?
Object:	Transient + V* (SIMBAD class: Variable* = Variable Star)
Note:	The Evryscope is a telescope array designed to open a new parameter space in optical astronomy, detecting short-timescale events across extremely large sky areas simultaneously. More information available at: http://evryscope.astro.unc.edu/ Format -CB-NNN: for compact binaries. Format -HSD-NNN: for candidate hot subdwarf binaries.
Ref:	=2019PASP..131g5001R
by	RATZLOFF J.K. , LAW N.M., FORS O., CORBETT H.T., HOWARD W.S., DEL SER D., HAISLIP J.
	PASP, 131g, 5001-75001 (2019)
	Building the Evryscope: hardware design and performance.
o	Tables 4-6: <EVR JHHMMSS.ss+DDMMSS.s> N=45+1+14.
Ref:	=2019PASP..131h4201R
by	RATZLOFF J.K. , CORBETT H.T., LAW N.M., BARLOW B.N., GLAZIER A., HOWARD W.S., FORS O., DEL SER D., TRIFONOV T.
	PASP, 131h, 4201-84201 (2019)
	Variables in the Southern polar region Evryscope 2016 data set.
o	Tables 8-11: <EVR JHHMMSS.ss+DDMMSS.s> N=6+3+135+159.
Ref:	=2019ApJ...883...51R
by	RATZLOFF J.K. , BARLOW B.N., KUPFER T., CORCORAN K.A., GEIER S., BAUER E., CORBETT H.T., HOWARD W.S., GLAZIER A., LAW N.M.
	Astrophys. J., 883, 51-51 (2019)
	EVR-CB-001: an evolving, progenitor, white dwarf compact binary discovered with the Evryscope.
o	<EVR -CB-NNN> (No. 001).
Ref:	=2020ApJ...890..126R
by	RATZLOFF J.K. , BARLOW B.N., NEMETH P., CORBETT H.T., WALSER S., GALLIHER N.W., GLAZIER A., HOWARD W.S., LAW N.M.
	Astrophys. J., 890, 126-126 (2020)
	Hot subdwarf all southern sky fast transit survey with the Evryscope.
o	Table 10: <EVR-HSD-NNN> N=18 among (Nos 001-024), <EVR-CB-NNN> (Nos 002-004) added. Table 11: <EVR JHHMMSS.ss+DDMMSS.s> N=14 added.
=E=	Catalogue in electronic form as <J/PASP/131/H4201/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EVS83]
[EVS83]	(Ekers+Van Gorkom+Schwarz+, 1983)
====>	Equivalent to: EVSG
Origin	of the Acronym: L (1987ApJ...320..545Y)
Details on Acronym: EVSG
EVSG	(Ekers+Van Gorkom+Schwarz+Goss)= [EVS83]
Write:	<<EVSG A>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	See also [HJB85]
in source:	NAME Sgr A
Ref:	=1983A&A...122..143E
by	EKERS R.D. , VAN GORKOM J.H., SCHWARZ U.J., GOSS W.M.
	Astron. Astrophys., 122, 143-150 (1983)
	The radio structure of Sgr A.
o	Table 2: <EVSG A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EWB86]
[EWB86]	(Eckart+Witzel+Biermann+, 1986)
Write:	<<[EWB86] S5 HHMM+DD A>> <<[EWB86] S5 HHMM+DD AN>>
N:	91
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Components of N=13 S5 radio-sources. Components 'A' are independent of the wavelength, components 'AN' are dependent of the wavelength: letter K, components 'KN': 1.3 cm. letter X, components 'XN': 2.8cm letter C, components 'CN': 6cm letter L,components 'LN': 18cm
Ref:	=1986A&A...168...17E
by	ECKART A. , WITZEL A., BIERMANN P., JOHNSTON K.J., SIMON R., SCHALINSKI C., KUHR H.
	Astron. Astrophys., 168, 17-24 (1986)
	Investigation of a complete sample of flat spectrum radio sources from the S 5 Survey. I. Analysis.
o	Table 4: <[EWB86] S5 HHMM+DD A> N=26.
Ref:	=1987A&AS...67..121E
by	ECKART A. , WITZEL A., BIERMANN P., JOHNSTON K.J., SIMON R., SCHALINSKI C., KUHR H.
	Astron. Astrophys., Suppl. Ser., 67, 121-146 (1987)
	Investigation of a complete sample of flat spectrum radio sources from the S5 survey. II. Results.
o	Table II: <[EWB86] S5 HHMM+DD A> = <[EWB86] S5 HHMM+DD AN> N=62 new.
Ref:	=1988A&A...206..245W
by	WITZEL A. , SCHALINSKI C.J., JOHNSTON K.J., BIERMANN P.L., KRICHBAUM T.P., HUMMEL C.A., ECKART A.
	Astron. Astrophys., 206, 245-252 (1988)
	The occurrence of bulk relativistic motion in compact radio sources.
o	Table 1: <[EWB86] S5 HHMM+DD CN> N=3 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EWM2010]
[EWM2010]	(Eskridge+Windhorst+Mager+, 2010) (Not yet in Simbad)
Write:	<<[EWM2010] NNNN>>
N:	4360
Object:	* (SIMBAD class: Star)
Note:	HST WFPC2 and NICMOS observations of NGC 1311.
in source:	NGC 1311
Ref:	=2010AJ....140.1137E
by	ESKRIDGE P.B. , WINDHORST R.A., MAGER V.A., JANSEN R.A.
	Astron. J., 140, 1137-1149 (2010)
	The young stellar population of the nearby late-type galaxy NGC 1311.
o	Table 3: <[EWM2010] NNNN> (Nos 1-4360).
=E=	Catalogue in electronic form as <J/AJ/140/1137/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EWM2011]
[EWM2011]	(Erickson+Wilking+Meyer+, 2011)
Write:	<<[EWM2011] F-NN>>
N:	219
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	CTIO Blanco/Hydra spectroscopy of N=219 stars in the ρ Oph Cloud.
in source:	NAME rho Oph Cloud
Ref:	=2011AJ....142..140E
by	ERICKSON K.L. , WILKING B.A., MEYER M.R., ROBINSON J.G., STEPHENSON L.N.
	Astron. J., 142, 140 (2011)
	The initial mass function and disk frequency of the ρ Ophiuchi cloud: an extinction-limited sample.
o	Tables 2-3: <[EWM2011] F-NN> N=219.
=E=	Catalogue in electronic form as J/AJ/142/140
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EWM2015]
[EWM2015]	(Erickson+Wilking+Meyer+, 2015)
Write:	<<[EWM2015] JHHMMSS.s+DDMMSS.s>>
N:	269
Object:	* (SIMBAD class: Star)
Note:	WIYN Hydra, Bok telescope B&C, MMT Hectospec, and Magellan Clay MIKE spectroscopy of N=269 stars in the Serpens Cluster.
in source:	NAME Serpens Cluster
Ref:	=2015AJ....149..103E
by	ERICKSON K.L. , WILKING B.A., MEYER M.R., KIM J.S., SHERRY W., FREEMAN M.
	Astron. J., 149, 103 (2015)
	An optical spectroscopic survey of the Serpens main cluster: evidence for two populations?
o	Table 2: <[EWM2015] JHHMMSS.s+DDMMSS.s> N=269.
=E=	Catalogue in electronic form as J/AJ/149/103
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EWN94]
[EWN94]	(Ellingsen+Whiteoak+Norris+, 1994)
Write:	<<[EWN94] HHMMSS.ss+DDMMSS.s>> <<[EWN94] HHMMSS.ss+DDMMSS>>
N:	2
Object:	CH3OH Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	N=2 masers respectively in [MBB72] 18 and 23 in the LMC. Maser in [MBB72] 23 was already cited in 1992MNRAS.256p..33S.
in source:	Magellanic Clouds:LMC:[MBB72] 18 = [MBB72] 18
in source:	Magellanic Clouds:LMC:[MBB72] 23 = [MBB72] 23
Ref:	=1994MNRAS.269.1019E
by	ELLINGSEN S.P. , WHITEOAK J.B., NORRIS R.P., CASWELL J.L., VAILE R.A.
	Mon. Not. R. Astron. Soc., 269, 1019-1024 (1994)
	A search for methanol masers in the Magellanic Clouds.
o	Text: <[EWN94] HHMMSS.ss+DDMMSS.s> N=1, <[EWN94] HHMMSS.ss+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EWS
EWS	(Early Warning System)= OGLE
Write:	<<OGLE YYYY-AAA-NNN>> <<OGLE YYYY-AAA-NNNN>>
Object:	Microlensing Event (SIMBAD class: LensingEv = (Micro)Lensing Event)
Note:	OGLE microlensing events, first named by the authors as OGLE NNa events in Galactic Bulge. Starting 1998, the year has been included in the format: 'YYYY-BUL-NNN' and the objects were at first designated 'EWS'. In other galaxies, events have the same format. For example, 1999-CAR-1 microlensing event observed in the Carina galaxy, or 2005-SMC-001 in the SMC. See the OGLE-IV Early Warning System webpage: http://ogle.astrouw.edu.pl/ogle4/ews/ews.html Only first refs are listed here.
in source:	NAME Galactic Bulge
in source:	NAME Carina Dwarf Galaxy
in source:	Magellanic Clouds:LMC = LMC
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1999A&A...350L..19M
by	MAO S.
	Astron. Astrophys., 350, 19-22 (1999)
	An ongoing parallax microlensing event OGLE-1999-CAR-1 toward Carina.
o	<OGLE-YYYY-AAA-NN> N=1 (No. 1999-CAR-01).
Ref:	=2000AcA....50....1U
by	UDALSKI A. , ZEBRUN K., SZYMANSKI M., KUBIAK M., PIETRZYNSKI G., SOSZYNSKI I., WOZNIAK P.
	Acta Astron., 50, 1-65 (2000)
	The Optical Gravitational Lensing Experiment. Catalog of microlensing events in the Galactic Bulge.
o	Table 2: <OGLE-YYYY-BUL-NN> N=84.
Ref:	=2003MNRAS.343.1131T
by	TSAPRAS Y. , HORNE K., KANE S., CARSON R.
	Mon. Not. R. Astron. Soc., 343, 1131-1144 (2003)
	Microlensing limits on numbers and orbits of extrasolar planets from the 1998-2000 OGLE events.
o	Table 1: <OGLE-1998-BUL-NN> N=37 among (Nos 01-41). Table 2: <OGLE-1999-BUL-NN> N=37 among (Nos 01-46). Table 3: <OGLE-2000-BUL-NN> N=72 among (Nos 01-75).
Ref:	=2003AcA....53..291U
by	UDALSKI A.
	Acta Astron., 53, 291-305 (2003)
	The optical gravitational lensing experiment. Real time data analysis systems in the OGLE-III survey.
o	Text: <OGLE-YYYY-BUL-NNN> N=5 added. Text: <OGLEIII YYYY-NOOS-NNN> N=6.
Ref:	=2006ApJ...637L..73K
by	KOCHANEK C.S. , MOCHEJSKA B., MORGAN N.D., STANEK K.Z.
	Astrophys. J., 637, 73-76 (2006)
	A simple method to find all lensed quasars.
o	<OGLE-YYYY-AAA-NNN> (No. 2005-SMC-001).
=E=	Catalogue in electronic form as J/AcA/50/1
=E=	Catalogue in electronic form as J/MNRAS/343/1131
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EWS2005]
[EWS2005]	(Eggers+Stone+Nelson+, 2005) (Not yet in Simbad)
Write:	<<[EWS2005] NGC NNNN NN>>
N:	16+46
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
Note:	HST STIS observations of the interacting system NGC 3994-3995.
in source:	NGC 3994
in source:	NGC 3995
Ref:	=2005AJ....129..136E
by	EGGERS D. , WEISTROP D., STONE A., NELSON C.H., HANCOCK M.
	Astron. J., 129, 136-147 (2005)
	Hubble space telescope observations of star-forming regions in NGC 3994/3995.
o	Table 2: <[EWS2005] NGC 3994 NN> (Nos 1-16). Table 3: <[EWS2005] NGC 3995 NN> (Nos 1-46).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EWW2008]
[EWW2008]	(Esimbek+Wu+Wang, 2008)
Write:	<<[EWW2008] NN>> <<[EWW2008] GALL+B.ba>> <<[EWW2008] LLL.l+BB.ba>>
N:	41
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	Purple Mountain Observatory Qinghai Station 13.7m telescope 13CO(1-0) line observations of N=41 massive cores. N=41 13CO massive cores. See also [SSS85] and [DBY94].
Ref:	=2008NewA...13..144E
by	ESIMBEK J. , WU Y., WANG Y.
	NewA, 13, 144-156 (2008)
	A mapping study of massive cores with 13CO J=1-0 line.
o	Table 1: <[EWW2008] NN> (Nos 1-41) = <[EWW2008] GALL+B.ba> N=20 + <[EWW2008] LLL.l+BB.ba> N=21.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EXE
EXE	(Eridanus X-ray Enhancement)
Write:	<<NAME EXE N>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Table 4, maps
Ref:	=1993ApJ...406...97B
by	BURROWS D.N. , SINGH K.P., NOUSEK J.A., GARMIRE G.P., GOOD J.
	Astrophys. J., 406, 97-111 (1993)
	A multiwavelength study of the Eridanus soft X-ray enhancement.
o	<NAME EXE N> N=2
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EXG
EXG	(Extragalactic Galaxy)
*****	Avoid the usage of EXG, prefer [VHS96]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EXG
EXG	(Extragalactic Galaxy)
*****	Avoid the usage of EXG, prefer [VHS97]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EXMM
EXMM	(EXTraS XMM)
Write:	<<EXMM JHHMMSS.s+DDMMSS>>
Object:	(X) + Transient (SIMBAD class: Transient = Transient Event)
Note:	The EXTraS (“Exploring the X-ray Transient and variable Sky”) transient catalogue contains X-ray sources which can be significantly detected by XMM-Newton EPIC in a short time interval but not by the analysis of the full observation. This happens to strongly variable sources that are too dim to emerge from the background of a long observation or that are bright enough only during periods of high particle background removed by the standard analysis. The catalogue is available at https://www88.lamp.le.ac.uk/extras/query/extras_transients
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EXMS
EXMS	(EXOSAT Medium Slew)
Write:	<<EXMS BHHMM+DDdA>>
N:	1208
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	A catalog of X-ray sources detected during slew manouvers by the European Space Agency's EXOSAT satellite between 1983 and 1986. Identifications are proposed for about 80/100 of the entries.
Ref:	=1999A&AS..134..287R
by	REYNOLDS A.P. , PARMAR A.N., HAKALA P.J., POLLOCK A.M.T., WILLIAMS O.R., PEACOCK A., TAYLOR B.G.
	Astron. Astrophys., Suppl. Ser., 134, 287-300 (1999)
	The EXOSAT Medium-Energy Slew Survey Catalog.
o	Tables 3, 4, 5: <EXMS BHHMM+DDdA> N=1208.
=E=	Catalogue in electronic form as J/A+AS/134/287
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EXO
EXO	(Exosat satellite)= (DD) = (EXOSAT)
Write:	<<EXO HHMM+DDd>> <<EXO HHMM.m+DDMM>> <<EXO HHMMSS+DDMM.m>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Ref:	=1984EXOSA...3....1A
by	ANDREWS D.
	EXOSAT Express, 3, 1-24 (1984)
	EXOSAT Satellite.
Ref:	=1991ApJ...378...77G
by	GIOMMI P. , TAGLIAFERRI G., BEUERMANN K., BRANDUARDI-RAYMONT G., BRISSENDEN R., GRASER U., MASON K.O., MITTAZ J.P.D., MURDIN P., POOLEY G., THOMAS H.-C., TUOHY I.
	Astrophys. J., 378, 77-92 (1991)
	The EXOSAT high galactic latitude survey.
o	Table1, 2: <EXO HHMM.m+DDMM> N=233
Ref:	=1996A&AS..115..395L
by	LU F.J. , LI T.P., SUN X.J., WU M., PAGE C.G.
	Astron. Astrophys., Suppl. Ser., 115, 395-400 (1996)
	X-ray map from the EXOSAT galactic plane survey and a direct demodulation technique.
o	The 14 EXOSAT sources, named 'DD' by authors, are EXO sources in SIMBAD.
o	<EXO HHMM+DDd> N=14.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EXOSAT
EXOSAT	(Exosat satellite)
*****	Avoid the usage of EXOSAT, prefer EXO
Details on Acronym: EXP1
EXP1	(EXPLORE project, I)
Write:	<<EXP1 JHHMM+DDaNNaNNNNN>>
Object:	* with Planet (SIMBAD class: Star)
Note:	EXPLORE project: Extrasolar Planet Occultation Research. Search for stellar systems with planets.
Ref:	=2003ApJ...582.1123M
by	MALLEN-ORNELAS G. , SEAGER S., YEE H.K.C., MINNITI D., GLADDERS M.D., MALLEN-FULLERTON G.M., BROWN T.M.
	Astrophys. J., 582, 1123-1140 (2003)
	The EXPLORE project. I. A deep search for transiting extrasolar planets.
o	<EXP1 JHHMM+DDaNNaNNNNN> N=3.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EXS
EXS	(EXITE Source)
Write:	<<EXS HHMM.m+DDMM>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	1st reference from this experiment. In this ref., N=1 (X) source. EXITE (Energetic X-ray Imaging Telescope Experiment) balloon borne experiment.
Ref:	=1993A&AS...97..155G
by	GRINDLAY J.E. , COVAULT C.E., MANANDHAR R.P.
	Astron. Astrophys., Suppl. Ser., 97, 155-158 (1993)
	EXITE observation of the galactic center : a new transient ?
o	<EXS HHMM.m+DDMM>, 1st reference from this experiment, N=1
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EXS
EXS	(EPIC X-ray Source)
*****	Avoid the usage of EXS, prefer [SD2005]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: EXSS
EXSS	(EINSTEIN Extended Source Survey)= ([OHG97])
Write:	<<EXSS HHMM.m +DDMM>>
N:	1325
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Einstein observations. Table 2: In 1997AJ....113.2134O, N=321 objects from the authors catalogue (N=1325)
Ref:	=1997AJ....113.2134O
by	OPPENHEIMER B.R. , HELFAND D.J., GAIDOS E.J.
	Astron. J., 113, 2134-2146 (1997)
	A survey of the EINSTEIN IPC Database for extended X-ray sources.
o	Table 2: <EXSS HHMM.m +DDMM> N=321 among 1325
=E=	Catalogue in electronic form as IX/18
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EY
EY	(Ellingson+Yee)
Write:	<<EY PKS HHMM+DDd NNN>> <<EY 3C NNN.N NNN>> <<EY 4C 57.15 NNN>> <<EY 5C 2.10 NNN>> <<EY QSO 1641+399 NNN>>
N:	388
Object:	G (SIMBAD class: Galaxy)
Note:	Table 3: G in 8 QSO named in Table 2. N=388 among more than 600. Finding charts. 1991PASP vol. 103p. 396 describe the faint galaxy photometry program (PPP) used to obtain the catalog.
in source:	PKS 0405-123
in source:	NAME PKS 1146-O37
in source:	QSO B1641+399
in source:	4C 57.15
in source:	3C 215
in source:	3C 275.1
in source:	3C 345
in source:	5C 2.10
Ref:	=1994ApJS...92...33E
by	ELLINGSON E. , YEE H.K.C.
	Astrophys. J., Suppl. Ser., 92, 33-52 (1994)
	A redshift survey in quasar fields. I. Photometric and spectroscopic catalog.
o	Table 3: <EY PKS HHMM-DDd NNN>, <EY 4C 57.15 NNN> <EY 3C NNN.N NNN> <EY 5C 2.10 NNN> <EY QSO 1641+399 NNN> N=388.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [EYB94]
[EYB94]	(Ellingson+Yee+Bechtold+, 1994)
Write:	<<[EYB94] PG 0043+039 N>> <<[EYB94] PKS HHMM+DDd N>> <<[EYB94] PKS 2251+11 N>> <<[EYB94] 3C NNN N>> <<[EYB94] 4C 37.43 N>>
N:	40
Object:	G (SIMBAD class: Galaxy)
Note:	Table 2: G in 9 QSO fields. The galaxies are not numbered in ref. 1994AJ....107.1219E but are found numbered later in the literature.
Ref:	=1994AJ....107.1219E
by	ELLINGSON E. , YEE H.K.C., BECHTOLD J., DOBRZYCKI A.
	Astron. J., 107, 1219-1226 (1994)
	Metal-line absorption at z(abs) about z(em) from associated galaxies.
o	Table 2: <[EYB94] PG 0043+039 N> (Nos 1-5), <[EYB94] PKS 0044+030 N> (Nos 1-5), <[EYB94] PKS 0405-123 N> (Nos 1-9), <[EYB94] PKS 2251+11 N> (Nos 1-3), <[EYB94] 3C 95 N> (No. 1), <[EYB94] 3C 263 N> (Nos 1-8), <[EYB94] 3C 273 N> (Nos 1-3), <[EYB94] 3C 351 N> (No. 1), <[EYB94] 4C 37.43 N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EYG2006]
[EYG2006]	(Enoch+Young+Glenn+, 2006)= (Bolo)
Write:	<<[EYG2006] Bolo NNN>>
N:	122
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	1.1mm continuum survey of the Perseus molecular cloud with 'Bolocam' at Caltech Submillimeter Observatory.
in source:	NAME Perseus Molecular Cloud
Ref:	=2006ApJ...638..293E
by	ENOCH M.L. , YOUNG K.E., GLENN J., EVANS II N.J., GOLWALA S., SARGENT A.I., HARVEY P., AGUIRRE J., GOLDIN A., HAIG D., HUARD T.L., LANGE A., LAURENT G., MALONEY P., MAUSKOPF P., ROSSINOT P., SAYERS J.
	Astrophys. J., 638, 293-313 (2006)
	Bolocam survey for 1.1mm dust continuum emission in the c2d Legacy clouds. I. Perseus.
o	Table 1: <[EYG2006] Bolo NNN> (Nos 1-122).
=E=	Catalogue in electronic form as J/ApJ/638/293
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EYG89]
[EYG89]	(Ellingson+Yee+Green+, 1989)
Write:	<<[EYG89] NNN>>
N:	169
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Table I: N=169 galaxies in the cluster associated with the quasar 3C 206. See also Paper II: [EGY91]
Ref:	=1989AJ.....97.1539E
by	ELLINGSON E. , YEE H.K.C., GREEN R.F., KINMAN T.D.
	Astron. J., 97, 1539-1549 (1989)
	Clusters of galaxies associated with quasars. I. 3C 206.
o	Table I: <[EYG89] NNN> (Nos 1-169).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EYG91]
[EYG91]	(Ellingson+Yee+Green, 1991)
Write:	<<[EYG91] HHMM+DDd NNN>> <<[EYG91] HHMM+DD NNN>> <<[EYG91] 4C DD.NN NNN>> <<[EYG91] 5C DD.NN NNN>> <<[EYG91] 3C NNN.N NNN>>
N:	8697
Object:	G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 3: galaxies in the field of N=63 optically faint QSOs.
Ref:	=1991ApJS...76..455E
by	ELLINGSON E. , YEE H.K.C., GREEN R.F.
	Astrophys. J., Suppl. Ser., 76, 455-470 (1991)
	Quasars and active galactic nuclei in rich environments. I. Fields surrounding optically faint quasars.
o	Table 3: <[EYG91] HHMM+DDd NNN>, <[EYG91] HHMM+DD NNN>, <[EYG91] 4C DD.NN NNN>, <[EYG91] 5C DD.NN NNN>, <[EYG91] 3C NNN NNN>, <[EYG91] 3C NNN.N NNN>, N=8697.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EYH2001]
[EYH2001]	(Ellison+Yan+Hook+, 2001)
Write:	<<[EYH2001] QSO JHHMM+DDMM abs N.NNN>> <<[EYH2001] BHHMM+DDda>>
N:	22
Object:	DLA
Note:	CORALS survey. Table 3: DLAs in 19 QSOs are identified. Among them 4 QSOs have Multiple Damped Lyman Alpha Systems (MDLA) designated as 'BHHMM+DDda' and 'BHHMM+DDdb'. See also [LE2003]
in source:	QSO B1251-407
in source:	PKS 1354-107
in source:	QSO B2314-409
Ref:	=2001A&A...379..393E
by	ELLISON S.L. , YAN L., HOOK I.M., PETTINI M., WALL J.V., SHAVER P.
	Astron. Astrophys., 379, 393-406 (2001)
	The CORALS survey. I: New estimates of the number density and gas content of damped Lyman α systems free from dust bias.
o	Table 3: <[EYH2001] QSO JHHMM+DDMM abs N.NNN> N=22. Text: <[EYH2001] BHHMM+DDda> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EYM2008]
[EYM2008]	(Ellison+York+Murphy+, 2008) (Not yet in Simbad)
Write:	<<[EYM2008] SDSS JHHMMSS.ss+DDMMSS.s abs N.NNNN>>
N:	9
Object:	DLA
Note:	ESO VLT observations of N=9 SDSS QSOs.
Ref:	=2008MNRAS.383L..30E
by	ELLISON S.L. , YORK B.A., MURPHY M.T., ZYCH B.J., SMITH A.M., SARRE P.J.
	Mon. Not. R. Astron. Soc., 383L, 30-34 (2008)
	Diffuse interstellar bands in z < 0.6 CaII absorbers.
o	Table 1: <[EYM2008] SDSS JHHMMSS.ss+DDMMSS.s abs N.NNNN> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EYP2008]
[EYP2008]	(Ellison+York+Pettini+, 2008) (Not yet in Simbad)
Write:	<<[EYP2008] QSO JHHMM+DDMM abs N.NNN>>
N:	10
Object:	DLA
Note:	N=10 DLA in 8 QSOs spectra.
Ref:	=2008MNRAS.388.1349E
by	ELLISON S.L. , YORK B.A., PETTINI M., KANEKAR N.
	Mon. Not. R. Astron. Soc., 388, 1349-1360 (2008)
	A search for damped Lyman α systems towards radio-loud quasars I: the optical survey.
o	In Chap 4.1 : TXS 1013+235 not identified in the TXS Survey.
o	Table 4: <[EYP2008] QSO JHHMM+DDMM abs N.NNN> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EZ2009]
[EZ2009]	(Eigenthaler+Zeilinger, 2009)
Write:	<<[EZ2009] NN>>
N:	34
Object:	Poss. Group of G (SIMBAD class: GroupG_Candidate = Group of Galaxies Candidate)
Stat:	is completely incorporated in Simbad
Note:	WHT ISIS and VLT VIMOS observations of N=34 fossil group candidates. Use of SDSS and RASS data.
Ref:	=2009AN....330..978E
by	EIGENTHALER P. , ZEILINGER W.W.
	AN, 330, 978-987 (2009)
	The properties of fossil groups of galaxies.
o	Tables 3-4: <[EZ2009] NN> (Nos 1-34).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EZ2010]
[EZ2010]	(Eigenthaler+Zeilinger, 2010)
Write:	<<[EZ2010] N5846 NN>>
N:	56
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Use of SDSS data to find low-luminosity galaxies in the NGC 5846 group.
in source:	NAME NGC 5846 GROUP
Ref:	=2010A&A...511A..12E
by	EIGENTHALER P. , ZEILINGER W.W.
	Astron. Astrophys., 511A, 12-12 (2010)
	Revisiting the low-luminosity galaxy population of the NGC 5846 group with SDSS.
o	Table 1: <[EZ2010] N5846 NN> (Nos 01-56).
=E=	Catalogue in electronic form as <J/A+A/511/A12/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [EZ2012]
[EZ2012]	(Eigenthaler+Zeilinger, 2012)
Write:	<<[EZ2012] NN>>
N:	40
Object:	G (SIMBAD class: Galaxy)
Note:	VLT VIMOS spectroscopy of N=40 members of RX J1548.9+0851.
in source:	RX J1548.0+0851
Ref:	=2012A&A...540A.134E
by	EIGENTHALER P. , ZEILINGER W.W.
	Astron. Astrophys., 540A, 134-134 (2012)
	RX J1548.9+0851, a fossil cluster?
o	Fig. 2, Table 4: <[EZ2012] NN> N=40 among (Nos 1-83).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: EZOA
EZOA	(EBHIS HI detection in the Zone of Avoidance)
Write:	<<EZOA JHHMM+DDA>>
N:	170
Object:	G (SIMBAD class: Galaxy)
Note:	The Effelsberg–Bonn HI Survey (EBHIS, 2011AN....332..637K) is a blind HI survey of the sky north of Dec=-5degrees, conducted with the Effelsberg 100m radio telescope. We extracted a catalogue of detections in the Zone of Avoidance (\|b\|<6degrees) and gave the source names the prefix EZOA, reminiscent of the HIZOA sources (detected in a blind survey with teh Parkes radiotelescope).
Ref:	=2019MNRAS.489.2907S
by	SCHRODER A.C. , FLOER L., WINKEL B., KERP J.
	Mon. Not. R. Astron. Soc., 489, 2907-2922 (2019)
	EZOA - a catalogue of EBHIS H I-detected galaxies in the northern Zone of Avoidance.
o	<EZOA JHHMM+DDA> N=170. South African Astronomical Observatory
=E=	Catalogue in electronic form as <J/MNRAS/489/2907/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: F
F	(Frogel+)
*****	Avoid the usage of F, prefer FBMC
Origin	of the Acronym: L = Found in the literature
Details on Acronym: F
F	(Feige)
*****	Avoid the usage of F, prefer Feige
Origin	of the Acronym: L = Found in the literature
Details on Acronym: F
F	(Ford+)
*****	Avoid the usage of F, prefer Ford
Origin	of the Acronym: L = Found in the literature
Details on Acronym: F
F	(Fairall)
*****	Avoid the usage of F, prefer Frl
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: F
F	(Felli)
*****	Avoid the usage of F, prefer GMR
Origin	of the Acronym: L = Found in the literature
Details on Acronym: F
F	(Fehrenbach+)
*****	Avoid the usage of F, prefer GV
Origin	of the Acronym: L = Found in the literature
Details on Acronym: F
F	(F region)
*****	Avoid the usage of F, prefer [ML88]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: F
F	(F region)
Write:	<<NAME F N REGION>>
N:	3
Object:	Region (SIMBAD class: Region = Region defined in the Sky)
Stat:	is completely incorporated in Simbad
Note:	See also stars in the F1 to F3 regions: [C73], [ML88].
Ref:	=1973MmRAS..77..223C
by	COUSINS A.W.J.
	Mem. R. Astron. Soc., 77, 223-None (1973)
	Revised zero points and UBV photometry in the Harvard E and F regions.
o	Data previously published in 1972MNSSA..31..127C.
o	<NAME FN REGION> (Nos F1-F3). Table IV: <[C73] F1 A> (Nos A-N, J missing), <[C73] F2 A> (Nos A-M, J missing), <[C73] F3 A> (Nos A-N, B, J missing).
Details on Acronym: F
F	(Fehrenbach)
*****	Avoid the usage of F, prefer PV
Origin	of the Acronym: L = Found in the literature
Details on Acronym: F
F	(Field *)
*****	Avoid the usage of F, prefer WKK
Origin	of the Acronym: L = Found in the literature
Details on Acronym: F03G
F03G	(FIRST '03 catalog radio Galaxy or component Group) (Not yet in Simbad)
Write:	<<F03G JHHMMSS.s+DDMMSS>>
N:	over 2000
Object:	Radio G (SIMBAD class: RadioG = Radio Galaxy)
Note:	Identification of various morphological types of galaxies in the FIRST Survey. Since the FIRST catalogs are catalogs of components, it would be useful to have coordinate and size estimates for various types of radio galaxies, e.g. Wide-Angle Tail, Narrow-Angle Tail, HYMORE, and Double-Doubles made up of multiple components. Proctor, D. D. 2002, J. Electron. Imaging, 12, 398 (2003JEI....12..398P) Low Resolution Pattern Recognition - Sorting Triples in the FIRST Database. Use of Morphological Annotations for Groups in the FIRST Database. While many of the groups have components identifiable as 'cores' and are thus in the FIRST catalog, for a significant fraction there is no identifiable radio component at the expected core position. See also FIRST.
Ref:	=2006ApJS..165...95P
by	PROCTOR D.D.
	Astrophys. J., Suppl. Ser., 165, 95-107 (2006)
	Comparing pattern recognition feature sets for sorting triples in the FIRST database.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
History	of this Acronym: replaced by FCG
Details on Acronym: F117
F117	(Field F117)
*****	Avoid the usage of F117, prefer Gilmore
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [F2000]
[F2000]	(Forbes, 2000)
Write:	<<[F2000] NN>>
N:	74
Object:	* in Assoc. (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	NAME ASS SER OB 2-
Ref:	=2000AJ....120.2594F
by	FORBES D.
	Astron. J., 120, 2594-2608 (2000)
	The Serpens OB2 association and its thermal "Chimney".
o	Tables 3, 5: <[F2000] NN> (Nos 1-74).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [F2002]
[F2002]	(Fox, 2002)
Write:	<<[F2002] ANN>>
N:	3+1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-I observations: 3 possible counterparts of GRB 020127 are found.
Ref:	=2002GCN..1249....1F
by	FOX D.W.
	GRB Coordinates Network, Circular Service, 1249, 1-None (2002)
	GRB020127: comparison of Chandra epochs and identification of possible count erparts.
o	<[F2002] ANN> (Nos A7, A14, A45, B16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [F2005]
[F2005]	(Fynbo, 2005)
Write:	<<[F2005] GRB 050319 abs N.NN>>
N:	1
Object:	Absorber
Note:	NOT ALFOSC observations of GRB 050319. Several absorption features are found, including strong Ly-alpha corresponding to z=3.24.
Ref:	=2005GCN..3136....1F
by	FYNBO J.P.U. , HJORTH J., JENSEN B.L., JAKOBSSON P., MOLLER P., NARANEN J.
	GRB Coordinates Network, Circular Service, 3136, 1-None (2005)
	GRB 050319: absorption redshift from the nordic optical telescope.
o	<[F2005] GRB 050319 abs N.NN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [F2007]
[F2007]	(Fish, 2007) (Not yet in Simbad)
Write:	<<[F2007] JHHMMSS.ssss+DDMMSS.sss>>
N:	10
Object:	OH Maser (SIMBAD class: Maser)
Note:	VLBA and GBT observations of OH maser in the region Gal 11.904-0.141.
in source:	GAL 011.904-00.141
Ref:	=2007ApJ...665L.159F
by	FISH V.L.
	Astrophys. J., 665L, 159-161 (2007)
	OH masers in G11.904-0.141.
o	G11.904-0.141 = GPSR5 11.903-0.141
o	Table 1: <[F2007] JHHMMSS.ssss+DDMMSS.sss> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [F2013]
[F2013]	(Froebrich, 2013)
Write:	<<[F2013] FN>>
N:	6
Object:	Poss. Cluster of * (SIMBAD class: Cluster*_Candidate = Cluster of Stars Candidate)
Note:	N=6 red supergiant cluster candidates . Use of 2MASS, UKIDSS and VVV data.
Ref:	=2013IJAA....3..161F
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: F2M
F2M	(FIRST+2MASS)
Write:	<<F2M JHHMMSS.ss+DDMMSS.s>>
N:	69+137+395
Object:	QSO + Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Note:	Combined radio and optical + IR observations of FIRST and 2MASS objects to search for QSOs.
Ref:	=2004ApJ...607...60G
by	GLIKMAN E. , GREGG M.D., LACY M., HELFAND D.J., BECKER R.H., WHITE R.L.
	Astrophys. J., 607, 60-75 (2004)
	FIRST-2MASS sources below the APM detection threshold: a population of highly reddened quasars.
o	Table 2: <F2M JHHMMSS.ss+DDMMSS.s> N=69.
Ref:	=2007ApJ...667..673G
by	GLIKMAN E. , HELFAND D.J., WHITE R.L., BECKER R.H., GREGG M.D., LACY M.
	Astrophys. J., 667, 673-703 (2007)
	The FIRST-2MASS Red Quasar Survey.
o	Tables 1, 2: <F2M JHHMMSS.ss+DDMMSS.s> N=137 added.
Ref:	=2012ApJ...757...51G
by	GLIKMAN E. , URRUTIA T., LACY M., DJORGOVSKI S.G., MAHABAL A., MYERS A.D., ROSS N.P., PETITJEAN P., GE J., SCHNEIDER D.P., YORK D.G.
	Astrophys. J., 757, 51 (2012)
	FIRST-2MASS red quasars: transitional objects emerging from the dust.
o	Table 1: <F2M JHHMMSS.ss+DDMMSS.s> N=395.
=E=	Catalogue in electronic form as J/ApJ/607/60
=E=	Catalogue in electronic form as J/ApJ/667/673
=E=	Catalogue in electronic form as <J/ApJ/757/51/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: F2MS
F2MS	(FIRST+2MASS+SDSS)
Write:	<<F2MS JHHMM+DDMM>> <<F2MS HHMM+DDMM>> (not recognised by Simbad, but found in literature)
N:	52
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	Red quasars from a survey combining the FIRST radio survey, the 2MASS Infrared Survey and the Sloan Digital Sky Survey. Keck ESI spectroscopic follow-up. See also [UBW2009].
Ref:	=2009ApJ...698.1095U
by	URRUTIA T. , BECKER R.H., WHITE R.L., GLIKMAN E., LACY M., HODGE J., GREGG M.D.
	Astrophys. J., 698, 1095-1109 (2009)
	The FIRST-2MASS red quasar survey. II. An anomalously high fraction of LoBALs in searches for dust-reddened quasars.
o	Table 1: <[UBW2009] NNN> (Nos 1-122). Tables 2-3: <F2MS JHHMM+DDMM> N=51+21.
=E=	Catalogue in electronic form as <J/ApJ/698/1095/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: F3D
F3D	(Fornax 3D)
Write:	<<F3D JHHMMSS.ss+DDMMSS.ss>>
N:	1484
Object:	Poss. PN (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=1484 planetary nebula candidates in 21 early-type galaxies in the Fornax cluster, using VLT MUSE IFS observations from the Fornax 3D project.
in source:	NAME Fornax Cluster
Ref:	=2020A&A...637A..62S
by	SPRIGGS T.W. , SARZI M., NAPIWOTZKI R., GALAN-DE ANTA P.M., VIAENE S., NEDELCHEV B., COCCATO L., CORSINI E.M., DE ZEEUW P.T., FALCON-BARROSO J., GADOTTI D.A., IODICE E., LYUBENOVA M., MARTIN-NAVARRO I., McDERMID R.M., PINNA F., VAN DE VEN G., ZHU L.
	Astron. Astrophys., 637A, 62-62 (2020)
	Fornax 3D project: Automated detection of planetary nebulae in the centres of early-type galaxies and first results.
o	Tables 4-5: <F3D JHHMMSS.ss+DDMMSS.ss> N=98+63.
Ref:	=2021A&A...653A.167S
by	SPRIGGS T.W. , SARZI M., GALAN-DE ANTA P.M., NAPIWOTZKI R., VIAENE S., NEDELCHEV B., COCCATO L., CORSINI E.M., FAHRION K., FALCON-BARROSO J., GADOTTI D.A., IODICE E., LYUBENOVA M., MARTIN-NAVARRO I., McDERMID R.M., MORELLI L., PINNA F., VAN DE VEN G., DE ZEEUW P.T., ZHU L.
	Astron. Astrophys., 653A, 167-167 (2021)
	The Fornax3D project: Planetary nebulae catalogue and independent distance measurements to Fornax cluster galaxies.
o	Tables A.1-A.36: <F3D JHHMMSS.ss+DDMMSS.ss> N=1484.
=E=	Catalogue in electronic form as <J/A+A/637/A62/>
=E=	Catalogue in electronic form as <J/A+A/653/A167/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: F3R
F3R	(Furst+Reich+Reich+Reif)= (Reich 3-)
Write:	<<F3R NNNN>>
N:	6495
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Maps of these objects are found in ref. 1990A&AS vol. 58 p. 197, 1990A&AS...85..633R and 1990A&AS...85..691F. A few duplicated entries.
Ref:	=1990A&AS...85..805F
by	FURST E. , REICH W., REICH P., REIF K.
	Astron. Astrophys., Suppl. Ser., 85, 805-811 (1990)
	A radio continuum survey of the Galactic Plane at 11 cm wavelength. IV. A list of 6483 small diameter sources.
o	<F3R NNNN>, N=6483
=E=	Catalogue in electronic form as J/A+AS/85/805
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [F54]
[F54]	(Fricke, 1954)
Write:	<<[F54] SF NN>> <<[F54] NF NN>>
N:	35+26
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=35 stars in a South Field (SF) near M 31. Table 2: N=26 stars in a North Field (NF) near M 31 Maps.
Ref:	=1954ZA.....34..137F
by	FRICKE W.
	Zeitschr. Astrophys., 34, 137-167 (1954)
	Die Intensitat und Farbverteilung im Andromeda-Nebel.
o	Table 1: <[F54] SF NN> (Nos 1-35). Table 2: <[F54] SF NN> (Nos 1-26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [F77]
[F77]	(Frolov, 1977) (Not yet in Simbad)
Write:	<<[F77] Frolov 1 NN>>
N:	27
Object:	* in Cl* (SIMBAD class: Star)
in source:	NAME Cl Frolov 1
Ref:	=1977IzPul.195...80F
by	FROLOV V.N.
	Izv. Glav. Astron. Obs., 195, 80-97 (1977)
	Photometry and proper motions of stars of four galactic clusters in Cassiopeia.
o	Table 4: <Cl* NGC 7788 F NN> (Nos 1-67). Table 6: <Cl* NGC 7790 F NN> (Nos 1-60). Table 10: <Cl* Berkeley 58 F NN> (Nos 1-46). Table 11: <[F77] Frolov 1 NN> (Nos 1-27).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [F79]
[F79]	(Frolov, 1979) (Not yet in Simbad)
Write:	<<[F79] Frolov 1 UBV NN>> <<[F79] Frolov 1 BV NN>>
N:	13+14
Object:	* in Cl* (SIMBAD class: Star)
in source:	NAME FROLOV 1
Ref:	=1979IzPul.196...69F
by	FROLOV V.N.
	Izv. Glav. Astron. Obs., 196, 69-78 (1979)
	Membership of four open clusters in Cassiopeia from new data.
o	Table 2: <Cl* NGC 7788 Fr 1-NN> (Nos 1-1 to 1-42), <Cl* NGC 7788 Fr 2-NN> (Nos 2-1 to 2-17). Table 4: <Cl* NGC 7790 Fr 1-NN> (Nos 1-1 to 1-57), <Cl* NGC 7790 Fr 2-NN> (Nos 2-1 to 2-28). Table 5: <Cl* Berkeley 58 Fr 1-NN> (Nos 1-1 to 1-26), <Cl* Berkeley 58 Fr 2-NN> (Nos 2-1 to 2-15). Table 6: <[F79] Frolov 1 UBV NN> (Nos 1-13), <[F79] Frolov 1 BV NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [F80]
[F80]	(Fairall, 1980)= (Fairall)
Write:	<<[F80] NN>>
N:	46
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Ref:	=1980MNRAS.191..391F
by	FAIRALL A.P.
	Mon. Not. R. Astron. Soc., 191, 391-397 (1980)
	Galaxies with strong narrow emission lines: spectroscopy, morphology and range in absolute sizes.
o	<[F80] NN> N=46
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [F81]
[F81]	(Fetisova, 1981)
Write:	<<[F81] NNN>>
N:	452
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Ref:	=1981SvA....25..647F
by	FETISOVA T.S.
	Sov. Astron., 25, 647-658 (1981)
	A catalog of galaxy clusters with measured redshifts.
o	Table 1: <[F81] NNN> (Nos 1-452)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: F867
F867	(Field F867)
*****	Avoid the usage of F867, prefer Gilmore
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [F88]
[F88]	(Fabbiano, 1988)= ([F88a]) = (X)
Write:	<<[F88] X-NN>>
N:	13
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Einstein IPC and HRI observations. See also: [FT84], [FT87], [TFP88], [TFR90], TF, [FKT92]
in source:	M 81 = NGC 3031
Ref:	=1988ApJ...325..544F
by	FABBIANO G.
	Astrophys. J., 325, 544-562 (1988)
	The X-ray emission of M 81 and its nucleus.
o	<[F88] X-NN> (Nos X-1 to X-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [F88a]
[F88a]	(Fabbiano, 1988)
*****	Avoid the usage of [F88a], prefer [F88]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [F88b]
[F88b]	(Freedman, 1988)
Write:	<<[F88b] N-NNNN>> <<[F88b] aN>> <<[F88b] aaN>>
N:	855+1369+39+31
Object:	* (SIMBAD class: Star)
Note:	Table II: stars in field 1, format '1-NNN', (Nos 1-1 to 1-855). Table III: stars in field 2, format '2-NNNN', (Nos 2-1 to 2-1369). Table IV(b): bright stars in field 1, with large CH I values, format 'a1' (Nos a1-z1), and format 'aa1' (Nos aa1-mm1). Table V(b): bright stars in field 2, with large CH I values, format 'a2' (Nos a2-z2), and format 'aa2' (Nos aa2-ee2). See also [F89], stars in M 32, [WFM90], stars in M 33.
in source:	IC 1613
Ref:	=1988AJ.....96.1248F
by	FREEDMAN W.L.
	Astron. J., 96, 1248-1306 (1988)
	Stellar content of nearby galaxies. I. BVRI CCD photometry for IC 1613.
o	Table II: <[F88b] 1-NNN> (Nos 1-855). Table III: <[F88b] 2-NNNN> (Nos 1-1369). Table IV(b): <[F88b] a1> (Nos a1-z1), <[F88b] aa1> (Nos aa1-mm1). Table V: <[F88b] a2> (Nos a2-z2), <[F88b] aa2> (Nos aa2-ee2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [F88c]
[F88c]	(Freedman, 1988)
Write:	<<[F88c] F1-NN>> <<[F88c] F2-NN>>
N:	28+52
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Note:	Table 2: candidate Cepheids in 2 CCD fields: field 1: format 'F1-NN', (Nos 1-28). field 2: format 'F2-NN', (Nos 1-52)
in source:	IC 1613
Ref:	=1988ApJ...326..691F
by	FREEDMAN W.L.
	Astrophys. J., 326, 691-709 (1988)
	New Cepheid distances to nearby galaxies based on BVRI CCD photometry. I. IC 1613.
o	Table 2A: <[F88c] F1-NN> (Nos 1-28). Table 2B: <[F88c] F2-NN> (Nos 1-52)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [F89]
[F89]	(Freedman, 1989)= ([F89a])
Write:	<<[F89] OF NNN>> <<[F89] IF NNN>>
N:	600+400
Object:	* (SIMBAD class: Star)
Note:	Table I: * in 'Outer Field', format 'OF NNN', (Nos 1-600). Table II: * in 'Inner Field', format 'IF NNN', (Nos 1-400). See also [F88b], * in IC 1613, [WFM90], * in M 33.
in source:	M 32
Ref:	=1989AJ.....98.1285F
by	FREEDMAN W.L.
	Astron. J., 98, 1285-1304 (1989)
	Stellar content of nearby galaxies. II. The local group dwarf elliptical galaxy M 32.
o	Table I: <[F89] OF NNN> (Nos 1-600). Table II: <[F89] IF NNN> (Nos 1-400)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [F89a]
[F89a]	(Freedman, 1989)
*****	Avoid the usage of [F89a], prefer [F89]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [F89b]
[F89b]	(Forbes, 1989) (Not yet in Simbad)
Write:	<<[F89b] SNNN N>>
N:	60
Object:	* (SIMBAD class: Star)
Note:	N=60 stars associated with 15 HII regions.
Ref:	=1989A&AS...77..439F
by	FORBES D.
	Astron. Astrophys., Suppl. Ser., 77, 439-445 (1989)
	Photometry and spectroscopy of stars in northern H II regions.
o	Table I: <[F89b] SNNN N> N=60.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [F90]
[F90]	(Fesen, 1990)
Write:	<<[F90] A>>
N:	5
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
in source:	NAME Cas A
Ref:	=1990AJ.....99.1904F
by	FESEN R.A.
	Astron. J., 99, 1904-1906 (1990)
	An [Ne III] image of the Cassiopeia A supernova remnant.
o	Fig.1: <[F90] A> (Nos A-E)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [F92]
[F92]	(Freedman, 1992)
Write:	<<[F92] NNN>>
N:	125
Object:	* (SIMBAD class: Star)
in source:	M 32
Ref:	=1992AJ....104.1349F
by	FREEDMAN W.L.
	Astron. J., 104, 1349-1359 (1992)
	Infrared-luminous giants in M32: an intermediate-age population?
o	<[F92] NNN> N=125
=E=	Catalogue in electronic form as J/AJ/104/1349
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [F94]
[F94]	(Falomo, 1994)
Write:	<<[F94] A>>
N:	3
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=3 knots in the optical jet of PKS 0521-365. See also [SUF99b].
in source:	PKS 0521-365
Ref:	=1994Msngr..77...49F
by	FALOMO R.
	The Messenger, 77, 49-52 (1994)
	High-resolution imaging of the active galaxy PKS 0521-365 and its optical jet.
o	Fig.5: <[F94] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [F97]
[F97]	(Feinstein, 1997)
Write:	<<[F97] NGC NNNN NNN>>
N:	1505
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Table 4: N=86 HII in NGC 1672. Table 5: N=373 HII in NGC 2997. Table 6: N=58 HII in NGC 4123. Table 7: N=45 HII in NGC 4593. Table 8: N=46 HII in NGC 4602. Table 9: N=174 HII in NGC 5364. Table 10: N=55 HII in NGC 5681. Table 11: N=62 HII in NGC 6070. Table 12: N=119 HII in NGC 6118. Table 13: N=283 HII in NGC 6384. Table 14: N=126 HII in NGC 7479. Table 15: N=78 HII in NGC 7552.
in source:	NGC 1672
in source:	NGC 2997
in source:	NGC 4123
in source:	NGC 4593
in source:	NGC 4602
in source:	NGC 5364
in source:	NGC 5681
in source:	NGC 6070
in source:	NGC 6118
in source:	NGC 6384
in source:	NGC 7479
in source:	NGC 7552
Ref:	=1997ApJS..112...29F
by	FEINSTEIN C.
	Astrophys. J., Suppl. Ser., 112, 29-47 (1997)
	H II regions in southern spiral galaxies: the Hα luminosity function.
o	Tables 4-15: <[F97] NGC NNNN NNN> N=1505
=E=	Catalogue in electronic form as J/ApJS/112/29
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [F98]
[F98]	(Festin, 1998)
Write:	<<[F98] omd NN>> <<[F98] serpmd N>> <<[F98] ophmd N>> <<[F98] owd N>> <<[F98] serpwd N>>
N:	21+7
Object:	Dw. * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	M dwarfs and white dwarfs ('md' and 'wd' in the format) in the area of Orion ('omd' and 'owd') N=11 and 3, in the area of Serpens ('serpmd' and 'serpwd') N=5+4, in the area of rho Oph ('ophmd') N=5
in source:	NAME Orion Nebula
in source:	NAME Serpens Nebula
in source:	NAME rho Oph Cloud
Ref:	=1998A&A...336..883F
by	FESTIN L.
	Astron. Astrophys., 336, 883-894 (1998)
	The luminosity function of white dwarfs and M dwarfs using dark nebulae as opaque outer screens.
o	Table 2: <[F98] omd NN> (Nos 1-11), <[F98] serpmd N> (Nos 1-5), <[F98] ophmd N> (Nos 1-5), <[F98] owd N> (Nos 1-3), <[F98] serpwd N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Fa
Fa	(Fairall)
*****	Avoid the usage of Fa, prefer Frl
Details on Acronym: [FA87]
[FA87]	(Forkert+Altschuler, 1987)
Write:	<<[FA87] HHMM+DDdA>>
N:	239
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Effelsberg radiotelescope observations at 2.7 and 4.75GHz.
Ref:	=1987A&AS...70...77F
by	FORKERT T. , ALTSCHULER D.R.
	Astron. Astrophys., Suppl. Ser., 70, 77-82 (1987)
	Flux density measurements of faint radio sources at 2.7 and 4.75 GHz.
o	Table III: <[FA87] HHMM+DDdA> N=239.
=E=	Catalogue in electronic form as VIII/57
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FAA2011]
[FAA2011]	(Faure+Anguita+Alloin+, 2011)
Write:	<<[FAA2011] DDD.ddddd+DD.ddddddd>> <<[FAA2011] COSMOS MMSS+MMSS AN>>
N:	27+34
Object:	G + Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	ESO VLT FORS1 spectroscopy of N=27 galaxies in the field of three COSMOS lens galaxies, and N=34 images in nine COSMOS lensing systems.
Ref:	=2011A&A...529A..72F
by	FAURE C. , ANGUITA T., ALLOIN D., BUNDY K., FINOGUENOV A., LEAUTHAUD A., KNOBEL C., KNEIB J.-P., JULLO E., ILBERT O., KOEKEMOER A.M., CAPAK P., SCOVILLE N., TASCA L.A.M.
	Astron. Astrophys., 529A, 72-72 (2011)
	On the evolution of environmental and mass properties of strong lens galaxies in COSMOS.
o	Table 2: <[FAA2011] DDD.ddddd+DD.ddddddd> N=27. Figs 7-11, Table 6: <[FAA2011] COSMOS MMSS+MMSS AN> N=34.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FAB2011]
[FAB2011]	(Foley+Andersson+Bazin+, 2011)
Write:	<<[FAB2011] DDD.ddddd+DD.ddddd>>
N:	18
Object:	G (SIMBAD class: Galaxy)
Note:	Magellan 6.5m telescope IMACS/GISMO and VLT FORS2 spectroscopy of galaxies in SPT-CL J2106-5844.
in source:	SPT-CL J2106-5844
Ref:	=2011ApJ...731...86F
by	FOLEY R.J. , ANDERSSON K., BAZIN G., DE HAAN T., RUEL J., ADE P.A.R., AIRD K.A., ARMSTRONG R., ASHBY M.L.N., BAUTZ M., BENSON B.A., BLEEM L.E., BONAMENTE M., BRODWIN M., CARLSTROM J.E., CHANG C.L., CLOCCHIATTI A., CRAWFORD T.M., CRITES A.T., DESAI S., DOBBS M.A., DUDLEY J.P., FAZIO G.G., FORMAN W.R., GARMIRE G., GEORGE E.M., GLADDERS M.D., GONZALEZ A.H., HALVERSON N.W., HIGH F.W., HOLDER G.P., HOLZAPFEL W.L., HOOVER S., HRUBES J.D., JONES C., JOY M., KEISLER R., KNOX L., LEE A.T., LEITCH E.M., LUEKER M., LUONG-VAN D., MARRONE D.P., McMAHON J.J., MEHL J., MEYER S.S., MOHR J.J., MONTROY T.E., MURRAY S.S., PADIN S., PLAGGE T., PRYKE C., REICHARDT C.L., REST A., RUHL J.E., SALIWANCHIK B.R., SARO A., SCHAFFER K.K., SHAW L., SHIROKOFF E., SONG J., SPIELER H.G., STALDER B., STANFORD S.A., STANISZEWSKI Z., STARK A.A., STORY K., STUBBS C.W., VANDERLINDE K., VIEIRA J.D., VIKHLININ A., WILLIAMSON R., ZENTENO A.
	Astrophys. J., 731, 86 (2011)
	Discovery and cosmological implications of SPT-CL J2106-5844, the most massive known cluster at z>1.
o	Table 1: <[FAB2011] DDD.ddddd+DD.ddddd> N=18.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FAB2017]
[FAB2017]	(Forbes+Alabi+Brodie+, 2017)
Write:	<<[FAB2017] NGCNNNN starNN>> <<[FAB2017] NGCNNNN galNN>> <<[FAB2017] NGCNNNN UCDNN>> <<[FAB2017] NGCNNNN SNNN>> <<[FAB2017] NGCNNNN GCNN>>
N:	580+285+33+3527+46
Object:	Star + G + UCD + GlCl (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Keck II DEIMOS and Subaru HSC observations of N=580+285 "contaminants" (stars and galaxies), N=33 ultra-compact dwarfs (UCDs), and N=3527+46 globular clusters, as part of the SLUGGS survey. Use of HST and CFHT imaging.
Ref:	=2017AJ....153..114F
by	FORBES D.A. , ALABI A., BRODIE J.P., ROMANOWSKY A.J., STRADER J., FOSTER C., USHER C., SPITLER L., BELLSTEDT S., PASTORELLO N., VILLAUME A., WASSERMAN A., POTA V.
	Astron. J., 153, 114-114 (2017)
	The SLUGGS survey: a catalog of over 4000 globular cluster radial velocities in 27 nearby early-type galaxies.
o	(Erratum) erratum vol. 154, art. 80 (2017)
o	Table 2: <[FAB2017] NGCNNNN starNN> N=580, <[FAB2017] NGCNNNN galNN> N=285. Table 4: <[FAB2017] NGCNNNN UCDNN> N=33. Table 5: <[FAB2017] NGCNNNN SNNN> N=3527, <[FAB2017] NGCNNNN GCNN> N=46.
=E=	Catalogue in electronic form as <J/AJ/153/114/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FAB2019]
[FAB2019]	(Forbes+Alabi+Brodie+, 2019)
Write:	<<[FAB2019] NGC 1052 GCNN>>
N:	77
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat.	in SIMBAD: NGC 1052 GC2 not in table A1
Note:	Keck II DEIMOS observations of N=77 globular clusters associated with NGC 1052.
in source:	NGC 1052
Ref:	=2019MNRAS.489.3665F
by	FORBES D.A. , ALABI A., BRODIE J.P., ROMANOWSKY A.J.
	Mon. Not. R. Astron. Soc., 489, 3665-3669 (2019)
	Dark matter and no dark matter: on the halo mass of NGC 1052.
o	Table A1: <[FAB2019] NGC 1052 GCNN> (Nos GC1-GC77).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FAB97]
[FAB97]	(Ferruit+Adam+Binette+, 1997) (Not yet in Simbad)
Write:	<<[FAB97] LV NN>> <<[FAB97] HV NN>>
N:	10+10
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Table 3, Fig.4: N=10 Low Velocity components of NGC 1275, format 'LV NN'. N=10 High Velocity components of NGC 1275, format 'HV NN.
in source:	NGC 1275 = 3C 84
Ref:	=1997NewA....2..345F
by	FERRUIT P. , ADAM G., BINETTE L., PECONTAL E.
	New Astronomy, 2, 345-363 (1997)
	Tiger observations of the low and high velocity components of NGC 1275.
o	Fig.17: Cluster 1 and 2 = [HFS92] 1 and 2
o	Table 3, Fig.4: <[FAB97] LV NN> (Nos 1-10), <[FAB97] HV NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FAE2003]
[FAE2003]	(Filipovic+Anderson+Ekers+, 2003)
Write:	<<[FAE2003] ATCA NN>> <<[FAE2003] ATCA JHHMMSS+DDMMSS>> <<[FAE2003] ROSAT NN>>
N:	93+85
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ATCA 20cm observations of the Deep Pavo Field. Comparison with ROSAT point sources.
in source:	NAME Deep Pavo Field
Ref:	=2003SerAJ.166...13F
by	FILIPOVIC M.D. , ANDERSON M., EKERS R.D., DANZIGER I.J., ZIMMERMANN H.-U., WHITE G.L., JONES P.A., BORUN B.C.P., PAYNE J.L., DIONNE M., GANIS M., OGNJANOVIC M.
	Serbian Astron. Journal, 166, 13-30 (2003)
	A multi-frequency study of the deep Pavo field.
o	Table 2: <[FAE2003] ATCA NN> (Nos 1-93) = <[FAE2003] ATCA JHHMMSS+DDMMSS> N=93. Table 3: <[FAE2003] ROSAT NN> (Nos 1-69).
=E=	Catalogue in electronic form as J/other/SerAJ/166.13
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FAG2003]
[FAG2003]	(Faure+Alloin+Gras+, 2003)
Write:	<<[FAG2003] N>> <<[FAG2003] VRN>>
N:	9+3
Object:	G (SIMBAD class: Galaxy)
Note:	VLT FORS1 and ISAAC and HST NICMOS2 observations. N=9 faint objects in the field of LBQS 1429-0053, and N=3 Very Red objects.
Ref:	=2003A&A...405..415F
by	FAURE C. , ALLOIN D., GRAS S., COURBIN F., KNEIB J.-P., HUDELOT P.
	Astron. Astrophys., 405, 415-424 (2003)
	LBQS 1429-0053: A binary quasar rather than a lensed quasar.
o	Figs 1-4, Table 2: <[FAG2003] N> (Nos 1-7), <[FAG2003] VRN> (Nos VR1-VR3).
Ref:	=2007ApJ...662L...1D
by	DJORGOVSKI S.G. , COURBIN F., MEYLAN G., SLUSE D., THOMPSON D., MAHABAL A., GLIKMAN E.
	Astrophys. J., 662L, 1-5 (2007)
	Discovery of a probable physical triple quasar.
o	In text, APM 08729+5255 is a misprint for APM 08279+5255
o	Text: <[DCM2007] QQQ J1432-0106> N=1, <[DCM2007] QSO JHHMM+DDMMA abs N.NNN>, <[DCM2007] QSO JHHMM+DDMMA abs N.NNNN>, N=2+2+1. Fig.1: <[FAG2003] N> (Nos 8, 9) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Fair
Fair	(Fairall)
*****	Avoid the usage of Fair, prefer Frl
Details on Acronym: Fairall
Fairall	(Fairall)
*****	Avoid the usage of Fairall, prefer [F80]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Fairall
Fairall	(Fairall)
*****	Avoid the usage of Fairall, prefer Frl
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [FAK2014]
[FAK2014]	(Foster+Arce+Kassis+, 2014)
Write:	<<[FAK2014] KN>> <<[FAK2014] A>>
N:	9+3
Object:	NIR + As* (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Keck II NIRC2 deep near-infrared observations of N=9 extended sources and N=3 overdensities within the filamentary Infrared Dark Cloud G34.43+00.24. Use of archival UKIDSS GPS data.
in source:	MSXDC G034.43+0.24
Ref:	=2014ApJ...791..108F
by	FOSTER J.B. , ARCE H.G., KASSIS M., SANHUEZA P., JACKSON J.M., FINN S.C., OFFNER S., SAKAI T., SAKAI N., YAMAMOTO S., GUZMAN A.E., RATHBORNE J.M.
	Astrophys. J., 791, 108 (2014)
	Distributed low-mass star formation in the IRDC G34.43+00.24.
o	Table 2: <[FAK2014] KN> (Nos K1-K9). Table 3: <[FAK2014] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Fan
Fan	(Fan+)
*****	Avoid the usage of Fan, prefer [FMZ2005]
Origin	of the Acronym: L (2007A&A...468...49V)
Details on Acronym: [FAP2012]
[FAP2012]	(Frolov+Ananjevskaja+Polyakov, 2012)
Write:	<<[FAP2012] NNNN>>
N:	1103
Object:	* (SIMBAD class: Star)
Note:	Astrometric catalog of N=1103 stars in the Galactic open cluster NGC 2323. Pulkovo normal astrograph observations from 1930-1990.
in source:	M 50 = NGC 2323
Ref:	=2012AstL...38...74F
by	FROLOV V.N. , ANANJEVSKAJA Y.K., POLYAKOV E.V.
	AstL, 38, 74-86 (2012)
	Investigation of the open star cluster NGC 2323 (M50) based on the proper motions and photometry of its constituent stars.
o	Table 3: <[FAP2012] NNNN> N=1103 among (Nos 1-1316).
o	2012PAZh...38...95F
=E=	Catalogue in electronic form as J/PAZh/38/95
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Farina
Farina
*****	Avoid the usage of Farina, prefer [FBM2009]
Origin	of the Acronym: L (2010AJ....139.1283W)
Details on Acronym: [FAS2003]
[FAS2003]	(Fujita+Ajiki+Shioya+, 2003)
Write:	<<[FAS2003] N-N>>
N:	6+2+8+7
Object:	Em. Obj. (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Note:	Survey of Lyman-alpha emission objects with the Subaru telescope in the Subaru/XMM-Newton Deep Field.. Table 2: Lyman-alpha emitter candidates at z about 3.7 Table 3: marginal Lyman-alpha emitter candidates. Table 4: low Lyman-alpha emitter candidates. Table 5: unclassified Lyman-alpha emitter candidates. In the format the first digit 'N' is the table number.
Ref:	=2003AJ....125...13F
by	FUJITA S.S. , AJIKI M., SHIOYA Y., NAGAO T., MURAYAMA T., TANIGUCHI Y., OKAMURA S., OUCHI M., SHIMASAKU K., DOI M., FURUSAWA H., HAMABE M., KIMURA M., KOMIYAMA Y., MIYAZAKI M., MIYAZAKI S., NAKATA F., SEKIGUCHI M., YAGI M., YASUDA N., MATSUDA Y., TAMURA H., HAYASHINO T., KODAIRA K., KAROJI H., YAMADA T., OHTA K., UMEMURA M.
	Astron. J., 125, 13-31 (2003)
	A search for Lyα emitters at redshift 3.7.
o	Table 2: <[FAS2003] 2-N> (Nos 2-1 to 2-6). Table 3: <[FAS2003] 3-N> (Nos 3-1 to 3-2). Table 4: <[FAS2003] 4-N> (Nos 4-1 to 4-8). Table 5: <[FAS2003] 5-N> (Nos 5-1 to 5-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FAS2014]
[FAS2014]	(Forbes+Almeida+Spitler+, 2014)
Write:	<<[FAS2014] NNN>>
N:	358
Object:	Poss. Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST ACS observations of N=358 star cluster system of NGC 1023.
in source:	NGC 1023
Ref:	=2014MNRAS.442.1049F
by	FORBES D.A. , ALMEIDA A., SPITLER L.R., POTA V.
	Mon. Not. R. Astron. Soc., 442, 1049-1053 (2014)
	Extended star clusters in NGC 1023 from HST/ACS mosaic imaging.
o	Table 1: <[FAS2014] NNN> N=358 among (Nos 1-377).
=E=	Catalogue in electronic form as J/MNRAS/442/1049
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FASHI
FASHI	(FAST All Sky HI Survey)
Write:	<<FASHI JHHMMSS.ss+DDMMSS.s>>
N:	41741 (SIMBAD class: HI = HI (21cm) Source)
Note:	The FAST All Sky HI Survey (FASHI) was designed to cover the entire FAST sky of ∼22000 square degrees between -14 and +66 deg declination and the frequency range 1000-1500MHz, and could eventually detect the H I emission of more than 100000 galaxies across the FAST detectable sky. From August 2020 to January 2023, FASHI observed and searched for 21cm HI emission in a sky area of more than 7600 square degrees with a median detection sensitivity of about 0.76 mJy/beam and a spectral line velocity resolution of ∼6.4 km/s. A total of 41741 extragalactic HI galaxies were detected in the frequency range 1305.5-1435.0MHz.
Ref:	=2024SCPMA..6719511Z
Auth.:	Chuan-Peng Zhang National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People's Republic of China
=E=	Catalogue in electronic form as <J/other/SCPMA/67.19511/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: FASTT
FASTT	(Flagstaff Astrometric Scanning Transit Telescope)= (HS)
Write:	<<FASTT NNNN>>
N:	1602
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	The Flagstaff Astrometric Scanning Transit Telescope is used to obtain astometric information in fields in support of the SDSS survey. 1998AJ....115..296H: N=1602 variable stars, (Nos 1-1602).
Ref:	=1998AJ....115..296H
by	HENDEN A.A. , STONE R.C.
	Astron. J., 115, 296-302 (1998)
	New variables in the sloan digital sky survey calibration fields.
o	Table 1: SDSS calibration regions not in SIMBAD. Tables 2, 3, col(2): internal designation numbering, not in SIMBAD
o	Table 1: <FASTT NNNN> (Nos 1-1602)
=E=	Catalogue in electronic form as J/AJ/115/296
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FAUST
FAUST	(Far UV Space Telescope)
*****	Avoid the usage of FAUST, prefer [BFA97]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: FAUST
FAUST	(Far UV Space Telescope)
*****	Avoid the usage of FAUST, prefer [BOA98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FAUST
FAUST	(Far UV Space Telescope)
*****	Avoid the usage of FAUST, prefer [DSB94]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: FAUST
FAUST	(Far UV Space Telescope)= (FSC) = (NGP)
Write:	<<FAUST NNNN>> <<FAUST NGP-NN>>
N:	4660+81
Object:	(Far UV) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	Observations of the FAUST telescope on ATLAS 1
Ref:	=1995ApJS...96..461B
by	BOWYER S. , SASSEEN T.P., WU X., LAMPTON M.
	Astrophys. J., Suppl. Ser., 96, 461-544 (1995)
	A catalog of far-ultraviolet point sources detected with the FAUST telescope on Atlas-1.
o	<FAUST NNNN> (Nos 1-4660)
Ref:	=1995ApJ...450..137B
by	BROSCH N. , ALMOZNINO E., LEIBOWITZ E.M., NETZER H., SASSEEN T.P., BOWYER S., LAMPTON M., WU X.
	Astrophys. J., 450, 137-148 (1995)
	A study of ultraviolet objects near the North Galactic Pole with FAUST.
o	The TD1 designations in the tables are NOT the standard ones.
o	<FAUST NGP-NN> (Nos 1-81)
=E=	Catalogue in electronic form as J/ApJS/96/461
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 1FAV
1FAV	(1FAVA)
Write:	<<1FAV JHHMM+DD>>
N:	215
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	N=215 flaring gamma-ray sources. Use of the analysis tool FAVA (Fermi All-sky Variability Analysis), to search for gamma-ray emitters in Fermi/LAT data.
Ref:	=2013ApJ...771...57A
by	ACKERMANN M. , AJELLO M., ALBERT A., ALLAFORT A., ANTOLINI E., BALDINI L., BALLET J., BARBIELLINI G., BASTIERI D., BECHTOL K., BELLAZZINI R., BLANDFORD R.D., BLOOM E.D., BONAMENTE E., BOTTACINI E., BOUVIER A., BRANDT T.J., BREGEON J., BRIGIDA M., BRUEL P., BUEHLER R., BUSON S., CALIANDRO G.A., CAMERON R.A., CARAVEO P.A., CAVAZZUTI E., CECCHI C., CHARLES E., CHEKHTMAN A., CHEUNG C.C., CHIANG J., CHIARO G., CIPRINI S., CLAUS R., COHEN-TANUGI J., CONRAD J., CUTINI S., DALTON M., D'AMMANDO F., DE ANGELIS A., DE PALMA F., DERMER C.D., DI VENERE L., DRELL P.S., DRLICA-WAGNER A., FAVUZZI C., FEGAN S.J., FERRARA E.C., FOCKE W.B., FRANCKOWIAK A., FUKAZAWA Y., FUNK S., FUSCO P., GARGANO F., GASPARRINI D., GERMANI S., GIGLIETTO N., GIORDANO F., GIROLETTI M., GLANZMAN T., GODFREY G., GRENIER I.A., GRONDIN M.-H., GROVE J.E., GUIRIEC S., HADASCH D., HANABATA Y., HARDING A.K., HAYASHIDA M., HAYS E., HEWITT J., HILL A.B., HORAN D., HOU X., HUGHES R.E., INOUE Y., JACKSON M.S., JOGLER T., JOHANNESSON G., JOHNSON W.N., KAMAE T., KATAOKA J., KAWANO T., KNODLSEDER J., KUSS M., LANDE J., LARSSON S., LATRONICO L., LEMOINE-GOUMARD M., LONGO F., LOPARCO F., LOTT B., LOVELLETTE M.N., LUBRANO P., MAYER M., MAZZIOTTA M.N., McENERY J.E., MICHELSON P.F., MITTHUMSIRI W., MIZUNO T., MONTE C., MONZANI M.E., MORSELLI A., MOSKALENKO I.V., MURGIA S., NEMMEN R., NUSS E., OHSUGI T., OKUMURA A., OMODEI N., ORIENTI M., ORLANDO E., ORMES J.F., PANEQUE D., PANETTA J.H., PERKINS J.S., PESCE-ROLLINS M., PIRON F., PIVATO G., PORTER T.A., RAINO S., RANDO R., RAZZANO M., REIMER A., REIMER O., ROMOLI C., ROTH M., SANCHEZ-CONDE M., SCARGLE J.D., SCHULZ A., SGRO C., SISKIND E.J., SPANDRE G., SPINELLI P., SUSON D.J., TAKAHASHI H., TAKEUCHI Y., THAYER J.G., THAYER J.B., THOMPSON D.J., TIBALDO L., TINIVELLA M., TORRES D.F., TOSTI G., TROJA E., TRONCONI V., USHER T.L., VANDENBROUCKE J., VASILEIOU V., VIANELLO G., VITALE V., WINER B.L., WOOD K.S., WOOD M., YANG Z.
	Astrophys. J., 771, 57 (2013)
	The Fermi all-sky variability analysis: a list of flaring γ-ray sources and the search for transients in our galaxy.
o	Table 1: <1FAV JHHMM+DD> N=215.
=E=	Catalogue in electronic form as J/ApJ/771/57
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 2FAV
2FAV	(2nd Fermi All-sky Variability Analysis Catalog)
Write:	<<2FAV JHHMM+DD.d>>
N:	about 518
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	The Fermi All-sky Variability Analysis (FAVA) is an analysis technique that searches for flaring sources in data collected by the Large Area Telescope (LAT) onboard NASA's Fermi Gamma-ray Space Telescope. It uses a photometric approach to blindly search for flares over the entire sky, and a likelihood analysis to precisely locate them and to measure their spectra. This catalog contains the flares and sources detected by running FAVA over the first 7.4 years of Fermi mission, from Modified Julian Date (MJD) 54682 (2008-08-04) to 57391 (2016-01-04). The analysis has been run in weekly time bin and in two independent energy bands, 100-800MeV and 0.8-300GeV. The detection threshold applied to the catalog flares is equivalent to 6sigma (pre trials).
Ref:	=2017ApJ...846...34A
by	ABDOLLAHI S. , ACKERMANN M., AJELLO M., ALBERT A., BALDINI L., BALLET J., BARBIELLINI G., BASTIERI D., BECERRA GONZALEZ J., BELLAZZINI R., BISSALDI E., BLANDFORD R.D., BLOOM E.D., BONINO R., BOTTACINI E., BREGEON J., BRUEL P., BUEHLER R., BUSON S., CAMERON R.A., CARAGIULO M., CARAVEO P.A., CAVAZZUTI E., CECCHI C., CHEKHTMAN A., CHEUNG C.C., CHIARO G., CIPRINI S., CONRAD J., COSTANTIN D., COSTANZA F., CUTINI S., D'AMMANDO F., DE PALMA F., DESAI A., DESIANTE R., DIGEL S.W., DI LALLA N., DI MAURO M., DI VENERE L., DONAGGIO B., DRELL P.S., FAVUZZI C., FEGAN S.J., FERRARA E.C., FOCKE W.B., FRANCKOWIAK A., FUKAZAWA Y., FUNK S., FUSCO P., GARGANO F., GASPARRINI D., GIGLIETTO N., GIOMI M., GIORDANO F., GIROLETTI M., GLANZMAN T., GREEN D., GRENIER I.A., GROVE J.E., GUILLEMOT L., GUIRIEC S., HAYS E., HORAN D., JOGLER T., JOHANNESSON G., JOHNSON A.S., KOCEVSKI D., KUSS M., LA MURA G., LARSSON S., LATRONICO L., LI J., LONGO F., LOPARCO F., LOVELLETTE M.N., LUBRANO P., MAGILL J.D., MALDERA S., MANFREDA A., MAYER M., MAZZIOTTA M.N., MICHELSON P.F., MITTHUMSIRI W., MIZUNO T., MONZANI M.E., MORSELLI A., MOSKALENKO I.V., NEGRO M., NUSS E., OHSUGI T., OMODEI N., ORIENTI M., ORLANDO E., PALIYA V.S., PANEQUE D., PERKINS J.S., PERSIC M., PESCE-ROLLINS M., PETROSIAN V., PIRON F., PORTER T.A., PRINCIPE G., RAINO S., RANDO R., RAZZANO M., RAZZAQUE S., REIMER A., REIMER O., SGRO C., SIMONE D., SISKIND E.J., SPADA F., SPANDRE G., SPINELLI P., STAWARZ L., SUSON D.J., TAKAHASHI M., TANAKA K., THAYER J.B., THOMPSON D.J., TORRES D.F., TORRESI E., TOSTI G., TROJA E., VIANELLO G., WOOD K.S.
	Astrophys. J., 846, 34-34 (2017)
	The second catalog of flaring γ-ray sources from the Fermi All-sky Variability Analysis.
o	Table 2: <2FAV JHHMM+DD.d> N=518. DESY, Zeuthen
=E=	Catalogue in electronic form as <J/ApJ/846/34/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: FB
FB	(Faint Blue)
Write:	<<FB NNN>>
N:	189
Object:	Blue * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1974ApJS...28..157G
by	GREENSTEIN J.L. , SARGENT A.I.
	Astrophys. J., Suppl. Ser., 28, 157-209 (1974)
	The nature of faint blue stars in the halo. II.
o	Tables A1 to A6: <FB NNN> (Nos 1-189)
Details on Acronym: FB
FB	(Far IR Background survey)
*****	Avoid the usage of FB, prefer FIRBACK
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [FB2003]
[FB2003]	(Frail+Berger, 2003)
Write:	<<[FB2003] JHHMMSS.sss+DDMMSS.ss>>
N:	1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA discovery of a radio source in the field of GRB 020819. This source is coincident with the host galaxy of the GRB (later confirmed in 2005ApJ...629...45J).
Ref:	=2003GCN..1842....1F
by	FRAIL D.A. , BERGER E.
	GRB Coordinates Network, Circular Service, 1842, 1-None (2003)
	GRB 020819: afterglow candidate.
o	<[FB2003] JHHMMSS.sss+DDMMSS.ss> N=1.
Details on Acronym: [FB2011]
[FB2011]	(Finkelman+Brosch, 2011)
Write:	<<[FB2011] NN>>
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Wise Observatory 1-m telescope narrowband Halpha observations of N=10 HII regions in UGC 4599. Use of SDSS data.
in source:	UGC 4599
Ref:	=2011MNRAS.413.2621F
by	FINKELMAN I. , BROSCH N.
	Mon. Not. R. Astron. Soc., 413, 2621-2632 (2011)
	UGC 4599: a photometric study of the nearest hoag-type ring galaxy.
o	Table 4: <[FB2011] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FB2017]
[FB2017]	(For+Bekki, 2017)
Write:	<<[FB2017] JDD.dddddd+DD.dddddd>>
N:	15
Object:	Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Note:	Detection of N=15 YSOs in LMC clusters. Use of HST HERITAGE band-matched and SC data.
Ref:	=2017MNRAS.468L..11F
by	FOR B.-Q. , BEKKI K.
	Mon. Not. R. Astron. Soc., 468L, 11-15 (2017)
	A discovery of young stellar objects in older clusters of the Large Magellanic Cloud.
o	Table 1: <[FB2017] JDD.dddddd+DD.dddddd> N=15.
Details on Acronym: [FB98]
[FB98]	(Frye+Broadhurst, 1998)
Write:	<<[FB98] Arc WN>>
N:	4+7
Object:	Arc (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	HST imaging and Keck spectroscopy of a z=4 galaxy lensed by ACO 2390.
in source:	ACO 2390
Ref:	=1998ApJ...499L.115F
by	FRYE B. , BROADHURST T.
	Astrophys. J., 499, 115-118 (1998)
	Discovery of red selected arcs at z = 4.04 behind Abell 2390.
o	The famous straight arc = [LPC98] 2 = [PLS91] Arc
o	text: <[FB98] Arc W> (Nos N, S, W, E) N=4
Ref:	=2000ApJ...531...95B
by	BUNKER A.J. , MOUSTAKAS L.A., DAVIS M.
	Astrophys. J., 531, 95-117 (2000)
	Resolving the stellar populations in a z=4 lensed galaxy.
o	Table 1: Offset star not in SIMBAD.
o	Table 1, Fig.3: <[FB98] Arc WN> (Nos N1-N4, S1-S3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBA2002]
[FBA2002]	(Formiggini+Brosch+Almoznino+, 2002)
Write:	<<[FBA2002] NNN>>
N:	228
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	UV image in the direction of Ophiuchus obtained with the FAUST instrument. See also FAUST.
in source:	NAME Oph Region
Ref:	=2002MNRAS.332..441F
by	FORMIGGINI L. , BROSCH N., ALMOZNINO E., BOWYER S., LAMPTON M.
	Mon. Not. R. Astron. Soc., 332, 441-455 (2002)
	Hidden subluminous stars among the FAUST UV sources towards Ophiuchus.
o	Some errors in the tables. See http://cdsweb.u-strasbg.fr/viz-bin/Vizie Rfor corrections.
o	Tables 1, 2: <[FBA2002] NNN> (Nos 1-228).
=E=	Catalogue in electronic form as J/MNRAS/332/441
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBB2002]
[FBB2002]	(Frye+Broadhurst+Benitez, 2002)
Write:	<<[FBB2002] ANNNN N>> <<[FBB2002] AC114 N>>
N:	3+1+3+1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=8 lensed galaxies at high redshift behind 4 massive clusters: ACO 1689, ACO 2390, ACO 2219, ACCG 114.
Ref:	=2002ApJ...568..558F
by	FRYE B. , BROADHURST T., BENITEZ N.
	Astrophys. J., 568, 558-575 (2002)
	Spectral evidence for widespread galaxy outflows at z > 4.
o	Table 1: <[FBB2002] A1689 N> (Nos 1-3), <[FBB2002] A2390 N> (No. 1), <[FBB2002] A2219 N> (Nos 1-3), <[FBB2002] AC114 N> (No. 1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBB2003]
[FBB2003]	(Forbes+Beasley+Bekki+, 2003)
Write:	<<[FBB2003] Spiral Galaxy>> <<[FBB2003] Dwarf Galaxy>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Note:	HST ACS observations. Discovery of a dwarf galaxy satellite of a edge-on spiral.
Ref:	=2003Sci...301.1217F
by	FORBES D.A. , BEASLEY M.A., BEKKI K., BRODIE J.P., STRADER J.
	Science, 301, 1217-1219 (2003)
	Galaxy disruption in a halo of dark matter.
o	<[FBB2003] Spiral Galaxy> N=1, <[FBB2003] Dwarf Galaxy> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBB2010]
[FBB2010]	(Fiocchi+Bassani+Bazzano+, 2010)
Write:	<<[FBB2010] IGR JHHMMm+DDMM NN>>
N:	21+8+10+1
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	N=21+8+10+1 X-ray sources, possible counterparts for INTEGRAL/IBIS sources. Use of Chandra/ACIS data archive.
in source:	IGR J10447-6027
in source:	IGR J12288+0052
in source:	IGR J12562+2554
in source:	IGR J16377-6423
Ref:	=2010ApJ...720..987F
by	FIOCCHI M. , BASSANI L., BAZZANO A., UBERTINI P., LANDI R., CAPITANIO F., BIRD A.J.
	Astrophys. J., 720, 987-995 (2010)
	Five new INTEGRAL unidentified hard X-ray sources uncovered by Chandra.
o	Table 2: <[FBB2010] IGR JHHMMm+DDMM NN> N=21+8+10+1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBB2011]
[FBB2011]	(Faherty+Burgasser+Bochanski+, 2011) (Not yet in Simbad)
Write:	<<[FBB2011] NLTT 20346/2MASS J0850+1057>> <<[FBB2011] NLTT 20346A>> <<[FBB2011] 2MASS J0850+1057>> <<[FBB2011] 2MASS J0850+1057A>>
N:	1+2+1+2
Object:	** + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	CTIO 4.0m Blanco telescope and LCO 6.5m Clay telescope observations of the multiple system NLTT 20346/2MASS J0850+1057. See also [BBG2011].
Ref:	=2011AJ....141...71F
by	FAHERTY J.K. , BURGASSER A.J., BOCHANSKI J.J., LOOPER D.L., WEST A.A., VAN DER BLIEK N.S.
	Astron. J., 141, 71 (2011)
	Identification of a wide, low-mass multiple system containing the brown dwarf 2MASS J0850359+105716.
o	<[FBB2011] NLTT 20346/2MASS J0850+1057> N=1. <[FBB2011] NLTT 20346A> (Nos A-B). <[FBB2011] 2MASS J0850+1057> N=1, <[FBB2011] 2MASS J0850+1057A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBB2012]
[FBB2012]	(Farina+Bosch+Barba, 2012)
Write:	<<[FBB2012] NNNN>> <<[FBB2012] DDD.ddddd+DD.ddddd>> <<[FBB2012] X>>
N:	3627+2+1
Object:	* + Poss. YSO + Region (SIMBAD class: Star)
Note:	Gemini-North NIRI observations of the giant star-forming region NGC 604 in M33.
in source:	NGC 604
Ref:	=2012AJ....143...43F
by	FARINA C. , BOSCH G.L., BARBA R.H.
	Astron. J., 143, 43 (2012)
	Unveiling the new generation of stars in NGC 604 with Gemini-NIRI.
o	Caption Figure 9 : NGC 2024 IRS 4 & S106 IRS24 do not exist, misprint for NGC 2024 IRS2 & S106 IRS4 (text p.6). WR NNa are DMS NGC 604 NNa ; knots A to F are [CG99b] NGC 604 A in Simbad.
o	Table 2: <[FBB2012] NNNN> N=3627 among (Nos 53-4427). Paragr. 3.2: <[FBB2012] DDD.ddddd+DD.ddddd> N=2. Fig. 10, Table 4: <[FBB2012] X> N=1.
=E=	Catalogue in electronic form as <J/AJ/143/43/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBB2012b]
[FBB2012b]	(Fusco+Buonanno+Bono+, 2012)
Write:	<<[FBB2012b] NNNNNN>>
N:	193051 (SIMBAD class: Star)
Note:	HST ACS observations of NGC 6822.
in source:	NGC 6822
Ref:	=2012A&A...548A.129F
by	FUSCO F. , BUONANNO R., BONO G., CASSISI S., MONELLI M., PIETRINFERNI A.
	Astron. Astrophys., 548A, 129-129 (2012)
	Distance and reddening of the Local Group dwarf irregular galaxy NGC 6822.
o	<[FBB2012b] NNNNNN> N=193051
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBB93]
[FBB93]	(Fernini+Burns+Bridle+, 1993)
Write:	<<[FBB93] 3C 55 FN>> <<[FBB93] 3C 265 A>> <<[FBB93] 3C 324 A>> <<[FBB93] 3C 356 A>>
N:	9+5+5+6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	N=24 radio components in 4 radio galaxies from the 3CR catalogue. See also [FBP97]
Ref:	=1993AJ....105.1690F
by	FERNINI I. , BURNS J.O., BRIDLE A.H., PERLEY R.A.
	Astron. J., 105, 1690-1709 (1993)
	Very large array imaging of five Fanaroff-Riley II 3CR radio galaxies.
o	Fig.3: <[FBB93] 3C 55 FN> (Nos F1-F8). Fig.4: <[FBB93] 3C 265 A> (Nos A-E). Fig.5: <[FBB93] 3C 324 A> (Nos A-E). Fig.6: <[FBB93] 3C 356 A> (Nos A-F).
Ref:	=1997AJ....114.2292F
by	FERNINI I. , BURNS J.O., PERLEY R.A.
	Astron. J., 114, 2292-2312 (1997)
	VLA imaging of Fanaroff-Riley II 3CR radio galaxies. II. Eight new images and comparisons with 3CR quasars.
o	in ref list: Garrington+ MNRAS.250.171 misprint for p. 271, Orr+ MNRAS.200 misprint for 100
o	Table 7: <[FBB93] 3C 55 F9> added. Fig.2: <[FBP97] 3C 20 A> (Nos A-E). Fig.5: <[FBP97] 3C 34 A> (Nos A-H). Fig.8: <[FBP97] 3C 42 A> (Nos A-D). Fig.10: <[FBP97] 3C 244.1 A> (Nos A-E). Fig.13: <[FBP97] 3C 252 A> (Nos A-E). Fig.16: <[FBP97] 3C 325 A> (Nos A-H). Fig.18-20: <[FBP97] 3C 330 A> (Nos A-F). Table 7: <[FBP97] 3C 22 A> (Nos A-B>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBB95]
[FBB95]	(Filippenko+Barth+Bower+, 1995)
Write:	<<[FBB95] A>> <<[FBB95] NN>>
N:	4+10
Object:	* + (Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST Wide Field Camera. (Nos A-D), N=4 reference stars. (Nos 1-11) objects near SN 1961V, No. 11 may be the survivor of SN 1961V.
Ref:	=1995AJ....110.2261F
by	FILIPPENKO A.V. , BARTH A.J., BOWER G.C., HO L.C.
	Astron. J., 110, 2261-2273 (1995)
	Was Fritz Zwicky's "type V" SN 1961V a guenuine supernova?
o	(Erratum) Erratum 1996, AJ 112, p. 806
o	Table 1: <[FBB95] A> (Nos A-D), Table 2: <[FBB95] NN> (Nos 1-10)
Ref:	=2002PASP..114..700V
by	VAN DYK S.D. , FILIPPENKO A.V., LI W.
	Publ. Astron. Soc. Pac., 114, 700-707 (2002)
	Possible recovery of SN 1961V in Hubble space telescope archival images.
o	Table 1, Fig.2: <[FBB95] NN> (No. 11) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBC2013]
[FBC2013]	(Fong+Berger+Chornock+, 2013) (Not yet in Simbad)
Write:	<<[FBC2013] GRB YYMMDDA GN>>
N:	1+1+5
Object:	G (SIMBAD class: Galaxy)
Note:	N=1+1+5 galaxies in the field of GRB 100625A, GRB 101219A and GRB 110112A, in the search for the host galaxies.
Ref:	=2013ApJ...769...56F
by	FONG W. , BERGER E., CHORNOCK R., MARGUTTI R., LEVAN A.J., TANVIR N.R., TUNNICLIFFE R.L., CZEKALA I., FOX D.B., PERLEY D.A., CENKO S.B., ZAUDERER B.A., LASKAR T., PERSSON S.E., MONSON A.J., KELSON D.D., BIRK C., MURPHY D., SERVILLAT M., ANGLADA G.
	Astrophys. J., 769, 56 (2013)
	Demographics of the galaxies hosting short-duration γ-ray bursts.
o	Figs 2+4+11: <[FBC2013] GRB YYMMDDA GN> N=1+1+5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBC2017]
[FBC2017]	(Foex+Bohringer+Chon, 2017)
Write:	<<[FBC2017] JHHMMSS.s+DDMMSS.s>>
N:	17293
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT VIMOS spectroscopy and ESO/MPG 2.2m telescope WFI photometry of N=17293 galaxies in N=10 galaxy clusters.
Ref:	=2017A&A...606A.122F
by	FOEX G. , BOHRINGER H., CHON G.
	Astron. Astrophys., 606A, 122-122 (2017)
	Comparison of hydrostatic and dynamical masses of distant X-ray luminous galaxy clusters.
o	Table D.1: <[FBC2017] JHHMMSS.s+DDMMSS.s> N=17293.
=E=	Catalogue in electronic form as J/A+A/606/A122
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBC99]
[FBC99]	(Fassnacht+Blandford+Cohen+, 1999)
Write:	<<[FBC99] 2045+265 A>> <<[FBC99] 2045+265 Galaxy>> <<[FBC99] 2045+265 Arc>>
N:	5+1+1
Object:	Component (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Gravitational lens CLASS B2045+265: N=5 components (Nos A-E), N=1 lens galaxy '2045+265 Galaxy' and N=1 Arc, '2045+265 Arc' in the system. See also [MKF2007].
in source:	CLASS B2045+265
Ref:	=1999AJ....117..658F
by	FASSNACHT C.D. , BLANDFORD R.D., COHEN J.G., MATTHEWS K., PEARSON T.J., READHEAD A.C.S., WOMBLE D.S., MYERS S.T., BROWNE I.W.A., JACKSON N.J., MARLOW D.R., WILKINSON P.N., KOOPMANS L.V.E., DE BRUYN A.G., SCHILIZZI R.T., BREMER M., MILEY G.
	Astron. J., 117, 658-670 (1999)
	B2045+265: a new four-image gravitational lens from CLASS.
o	Phase calibrator = QSO J2115+295. Standard star SJ 9184 not identified.
o	Table 2: <[FBC99] 2045+265 A> (Nos A-E). Table 5: <[FBC99] 2045+265 Galaxy> N=1, <[FBC99] 2045+265 Arc> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBD2002]
[FBD2002]	(Fasano+Bettoni+D'Onofrio+, 2002)
Write:	<<[FBD2002] ACO NNNN aNN>> <<[FBD2002] DC 2103-39 aNN>>
N:	312
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	N=312 early-type galaxies in seven clusters.
in source:	ACO 2151
in source:	ACO 119
in source:	ACO 1069
in source:	ACO 1983
in source:	ACO 2670
in source:	ACO 3125
in source:	DRCG 2103-39
Ref:	=2002A&A...387...26F
by	FASANO G. , BETTONI D., D'ONOFRIO M., KJAERGAARD P., MOLES M.
	Astron. Astrophys., 387, 26-39 (2002)
	The scaling relations of early-type galaxies in clusters. I. Surface photometry in seven nearby clusters.
o	Table 7: <[FBD2002] ACO NNNN aNN>, <[FBD2002] DC 2103-39 aNN>, N=312.
=E=	Catalogue in electronic form as J/A+A/387/26
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBD2005]
[FBD2005]	(Figueredo+Blum+Damineli+, 2005) (Not yet in Simbad)
Write:	<<[FBD2005] NNN>>
N:	17
Object:	* in Cl* (SIMBAD class: Star)
Note:	OSIRIS images at the CTIO have detected an OB star cluster in the giant HII region [WMG70] 333.1-00.4. Among the 866 stars detected, 17 have YSOs properties.
in source:	[WMG70] 333.1-00.4 = GAL 333.1-00.4
Ref:	=2005AJ....129.1523F
by	FIGUEREDO E. , BLUM R.D., DAMINELI A., CONTI P.S.
	Astron. J., 129, 1523-1533 (2005)
	The stellar content of obscured galactic giant H II regions. V. G333.1-0.4.
o	Figs 1, Tables 1-3, text: <[FBD2005] NNN> N=17 among 866.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBD2008]
[FBD2008]	(Figueredo+Blum+Damineli+, 2008) (Not yet in Simbad)
Write:	<<[FBD2008] NNN>> <<[FBD2008] ObjN>>
N:	22+3
Object:	* (SIMBAD class: Star)
Note:	Spectroscopc observations of W 51A.
in source:	W 51:W 51A = W 51A
Ref:	=2008AJ....136..221F
by	FIGUEREDO E. , BLUM R.D., DAMINELI A., CONTI P.S., BARBOSA C.L.
	Astron. J., 136, 221-233 (2008)
	The stellar content of obscured galactic giant H II regions. VI. W51A.
o	G 25.2-1.74 is a misprint for G 35.2-1.74.
o	Table 1: <[FBD2008] NNN> N=22 among (Nos 7-754). Fig.9: <[FBD2008] ObjN> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBD2011]
[FBD2011]	(Fujinaga+Bamba+Dotani+, 2011)
Write:	<<[FBD2011] A>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Suzaku XIS observations of the field of the gamma-ray source HESS J1702-420.
in source:	HESS J1702-420
Ref:	=2011PASJ...63S.857F
by	FUJINAGA T. , BAMBA A., DOTANI T., OZAKI M., PUHLHOFER G., WAGNER S., REIMER O., FUNK S., HINTON J.
	PASJ, 63S, 857-864 (2011)
	Suzaku observation of the unidentified very high energy γ-ray source HESS J1702-420.
o	Fig. 2, Table 2: <[FBD2011] A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FBDC
FBDC	(Figueredo+Blum+Daminelli+Conti)
Write:	<<FBDC NNNa>>
N:	25+3
Object:	* (SIMBAD class: Star)
Note:	Stars in the field of NGC 3576, possible members of an embedded cluster. See also [BDC99], [BDC2001], [FBD2002].
Ref:	=2002AJ....124.2739F
by	FIGUEREDO E. , BLUM R.D., DAMINELI A., CONTI P.S.
	Astron. J., 124, 2739-2748 (2002)
	The stellar content of obscured galactic giant H II regions. IV. NGC 3576.
o	Fig.1, Table 2: <FBDC NNN> N=25 among 315.
Ref:	=2003AJ....126.2411B
by	BARBOSA C.L. , DAMINELI A., BLUM R.D., CONTI P.S.
	Astron. J., 126, 2411-2420 (2003)
	Gemini mid-infrared imaging of massive young stellar objects in NGC 3576.
o	IRS 1 = [FP74] RCW 57 IRS 1
o	Table 4: <FBDC NNNa> N=3 added.
Origin	of the Acronym: L (2003AJ....126.2411B)
Details on Acronym: [FBF2023]
[FBF2023]	(Finkelstein+Bagley+Ferguson+, 2023)
Write:	<<[FBF2023] CEERSN NNNN>> <<[FBF2023] CEERSN_NNNN>> (not recognised by Simbad, but found in literature)
N:	26+38
Object:	Poss. G (SIMBAD class: Galaxy)
Note:	JWST NIRCam observations of N=26+38 galaxy candidates and spurious sources in the CANDELS Extended Groth Strip (EGS) field, as part of the Cosmic Evolution Early Release Science (CEERS) survey.
in source:	NAME Extended Groth Strip
Ref:	=2023ApJ...946L..13F
by	FINKELSTEIN S.L. , BAGLEY M.B., FERGUSON H.C., WILKINS S.M., KARTALTEPE J.S., PAPOVICH C., YUNG L.Y.A., ARRABAL HARO P., BEHROOZI P., DICKINSON M., KOCEVSKI D.D., KOEKEMOER A.M., LARSON R.L., LE BAIL A., MORALES A.M., PEREZ-GONZALEZ P.G., BURGARELLA D., DAVE R., HIRSCHMANN M., SOMERVILLE R.S., WUYTS S., BROMM V., CASEY C.M., FONTANA A., FUJIMOTO S., GARDNER J.P., GIAVALISCO M., GRAZIAN A., GROGIN N.A., HATHI N.P., HUTCHISON T.A., JHA S.W., JOGEE S., KEWLEY L.J., KIRKPATRICK A., LONG A.S., LOTZ J.M., PENTERICCI L., PIEREL J.D.R., PIRZKAL N., RAVINDRANATH S., RYAN R.E.Jr, TRUMP J.R., YANG G., BHATAWDEKAR R., BISIGELLO L., BUAT V., CALABRO A., CASTELLANO M., CLERI N.J., COOPER M.C., CROTON D., DADDI E., DEKEL A., ELBAZ D., FRANCO M., GAWISER E., HOLWERDA B.W., HUERTAS-COMPANY M., JASKOT A.E., LEUNG G.C.K., LUCAS R.A., MOBASHER B., PANDYA V., TACCHELLA S., WEINER B.J., ZAVALA J.A.
	Astrophys. J., 946L, 13 (2023)
	CEERS Key Paper. I. An Early Look into the First 500 Myr of Galaxy Formation with JWST.
o	Figs 4+19+20, Tables 2+4+5+6: <[FBF2023] CEERSN NNNN> N=26+38.
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: FBFTA
FBFTA	(Fehrenbach+Burnage+Figuiere+Traversa+Agniel)
Write:	<<FBFTA Per I NNN>> <<FBFTA Per II NNN>>
N:	128+130
Object:	* (SIMBAD class: Star)
Note:	Table II: * in the field Per I, format 'Per I NNN', N=128. Table III: * in the field Per II, format 'Per II NNN', N=130
Ref:	=1987A&AS...68..515F
by	FEHRENBACH C. , BURNAGE R., FIGUIERE J., TRAVERSA G., AGNIEL C.
	Astron. Astrophys., Suppl. Ser., 68, 515-520 (1987)
	Mesures de 258 vitesses radiales dans 2 champs situes pres de α Persee.
o	(Erratum) + erratum vol 71, 185
o	Table II: <FBFTA Per I NNN> N=128, Table III: <FBFTA Per II NNN> N=130
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FBG
FBG	(Fasen+Becker+Goodrich)
*****	Avoid the usage of FBG, prefer KB
Origin	of the Acronym: L (1996ApJ...470..967F)
Details on Acronym: [FBG2002]
[FBG2002]	(Feigelson+Broos+Gaffney+, 2002)= (Feigelson)
Write:	<<[FBG2002] NNNN>>
N:	1075
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of Ori Nebula.
in source:	NAME Orion Nebula
Ref:	=2002ApJ...574..258F
by	FEIGELSON E.D. , BROOS P., GAFFNEY III J.A., GARMIRE G., HILLENBRAND L.A., PRAVDO S.H., TOWNSLEY L., TSUBOI Y.
	Astrophys. J., 574, 258-292 (2002)
	X-ray-emitting young stars in the Orion nebula.
o	Table 2: <[FBG2002] NNNN> (Nos 1-1075) = <CXOONC JHHMMSS.s+DDMMSS> N=1075.
=E=	Catalogue in electronic form as J/ApJ/574/258
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBG2007]
[FBG2007]	(Federici+Bellazzini+Galleti+, 2007)
Write:	<<[FBG2007] NNNN>>
N:	1662
Object:	* in Cl* (SIMBAD class: Star)
Note:	HST ACS observations of the globular cluster Bol 514 in M 31.
in source:	M 31:Bol 514 = Bol 514
Ref:	=2007A&A...473..429F
by	FEDERICI L. , BELLAZZINI M., GALLETI S., FUSI PECCI F., BUZZONI A., PARMEGGIANI G.
	Astron. Astrophys., 473, 429-436 (2007)
	The extended structure of the remote cluster B514 in M 31. Detection of extra-tidal stars.
o	Table 5: <[FBG2007] NNNN> (Nos 1-1662).
=E=	Catalogue in electronic form as J/A+A/473/429
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBH2000]
[FBH2000]	(Filho+Barthel+Ho, 2000)
Write:	<<[FBH2000] NGC NNNN WW>>
N:	6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=6 sources in the fields of 6 galaxies. See also [FBH2002].
Ref:	=2000ApJS..129...93F
by	FILHO M.E. , BARTHEL P.D., HO L.C.
	Astrophys. J., Suppl. Ser., 129, 93-110 (2000)
	The nature of composite LINER/H II galaxies as revealed from high-resolution VLA observations.
o	Table 3: <[FBH2000] NGC 3593 N>, <[FBH2000] NGC 3684 SW>, <[FBH2000] NGC 4013 SE>, <[FBH2000] NGC 4424 SE>, <[FBH2000] NGC 4710 E>, <[FBH2000] NGC 5838 S>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBH2002]
[FBH2002]	(Filho+Barthel+Ho, 2002)
Write:	<<[FBH2002] IC NNNN WW>> <<[FBH2002] NGC NNNN WW>>
N:	8
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA observations. N=8 sources in the fields of 6 galaxies. See also [FBH2000].
Ref:	=2002ApJS..142..223F
by	FILHO M.E. , BARTHEL P.D., HO L.C.
	Astrophys. J., Suppl. Ser., 142, 223-238 (2002)
	The radio properties of composite LINER/H II galaxies.
o	(Erratum) erratum vol. 244, p. 223 (2003)
o	Table 3: <[FBH2002] IC NNNN WW>, <[FBH2002] NGC NNNN WW>, N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBH2004]
[FBH2004]	(Finoguenov+Briel+Henry+, 2004)
Write:	<<[FBH2004] XNNN>> <<[FBH2004] SNNN>>
N:	73+33
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton survey of the Coma Cluster.
in source:	Coma Cluster = ACO 1656
Ref:	=2004A&A...419...47F
by	FINOGUENOV A. , BRIEL U.G., HENRY J.P., GAVAZZI G., IGLESIAS-PARAMO J., BOSELLI A.
	Astron. Astrophys., 419, 47-61 (2004)
	The X-ray luminosity function of galaxies in the Coma cluster.
o	Table 1: <[FBH2004] XNNN> N=73 among (Nos X19-X569). Table 2: <[FBH2004] SNNN> N=33 among (Nos S6-S149).
=E=	Catalogue in electronic form as J/A+A/419/47
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBK98]
[FBK98]	(Ferrarese+Bresolin+Kennicutt+, 1998)
Write:	<<[FBK98] CNN>> <<[FBK98] VNN>> <<[FBK98] JHHMMSS.ss+DDMMSS.s>>
N:	34+23+8
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations. Table 5: (Nos C1-C34), Cepheids in NGC 2541. Tables 12, 15: (Nos V1-V23), V* in NGC 2541. Identif. charts Figs 5, 11. Map Fig. 4. See also: [FHM94], [HST94], [KIF96], [FFH96], [SHM96], [GPF97], [RMM97], [HHH98], [PSF98], [TFS98], [GHS99], [KIS99], [SHF99], [GFF99], [MHS99], [SFK99], [PKB99], [GSF2000], [MHS2000] Tables 17-20: Format 'JHHMMSS.ss+DDMMSS.s', N=8 secondary standards.
in source:	NGC 2541
Ref:	=1998ApJ...507..655F
by	FERRARESE L. , BRESOLIN F., KENNICUTT R.C.Jr, SAHA A., STETSON P.B., FREEDMAN W.L., MOULD J.R., MADORE B.F., SAKAI S., FORD H.C., GIBSON B.K., GRAHAM J.A., HAN M., HOESSEL J.G., HUCHRA J., HUGHES S.M., ILLINGWORTH G.D., PHELPS R., PROSSER C.F., SILBERMANN N.A.
	Astrophys. J., 507, 655-690 (1998)
	The Hubble space telescope key project on the extragalactic distance scale. XII. The discovery of cepheids and a new distance to NGC 2541.
o	Table 5: <[FBK98] CNN> (Nos C1-C34). Tables 12, 15: <[FBK98] VNN> (Nos V1-V23). Tables 17-20: <[FBK98] JHHMMSS.ss+DDMMSS.s> N=8.
=E=	Catalogue in electronic form as J/ApJ/507/655
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBL2008]
[FBL2008]	(Fassbender+Bohringer+Lamer+, 2008)
Write:	<<[FBL2008] A>> <<[FBL2008] JHHMM.m+DDMM>>
N:	2
Object:	Cl of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Detection of N=2 new cluster of galaxies in archival XMM-Newton data.
Ref:	=2008A&A...481L..73F
by	FASSBENDER R. , BOEHRINGER H., LAMER G., MULLIS C.R., ROSATI P., SCHWOPE A., KOHNERT J., SANTOS J.S.
	Astron. Astrophys., 481L, 73-77 (2008)
	Indications for 3Mpc-scale large-scale structure associated with an X-ray luminous cluster of galaxies at z=0.95.
o	Table 1: <[FBL2008] A> (Nos A-B) = <[FBL2008] JHHMM.m+DDMM> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBL2011]
[FBL2011]	(Filho+Brinchmann+Lobo+, 2011)
Write:	<<[FBL2011] NNNNN Aa>> <<[FBL2011] NNNNN AN>>
N:	28+26
Object:	(IR) + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT HAWK-I observations of N=8 maxBCG galaxy clusters. Use of SDSS and Stripe 82 archival data.
Ref:	=2011A&A...536A..35F
by	FILHO M.E. , BRINCHMANN J., LOBO C., ANTON S.
	Astron. Astrophys., 536A, 35-35 (2011)
	Optically faint radio sources: reborn AGN?
o	Tables 3,4 : <[FBL2011] NNNNN Aa> ; <[FBL2011] NNNNN AN> N=28+26
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBM2002]
[FBM2002]	(Frail+Bertoldi+Moriarty-Schieven+, 2002)
Write:	<<[FBM2002] A>> <<[FBM2002] SMM JHHMMm+DDMM>>
N:	5+1
Object:	G + * (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	(mm) and (submm) observations toward GRB 010222. N=4 galaxies (Nos A-D) and N=1 star (No. E). N=1 (submm) source, a dusty galaxy, host of GRB 010222.
Ref:	=2002ApJ...565..829F
by	FRAIL D.A. , BERTOLDI F., MORIARTY-SCHIEVEN G.H., BERGER E., PRICE P.A., BLOOM J.S., SARI R., KULKARNI S.R., GERARDY C.L., REICHART D.E., DJORGOVSKI S.G., GALAMA T.J., HARRISON F.A., WALTER F., SHEPHERD D.S., HALPERN J., PECK A.B., MENTEN K.M., YOST S.A., FOX D.W.
	Astrophys. J., 565, 829-835 (2002)
	GRB 010222: a burst within a starburst.
o	p. 831 ERO J164502+4626.4 = [HR94] 10
o	Fig.3, Table 2: <[FBM2002] A> (Nos A-E). Text: <[FBM2002] SMM JHHMMm+DDMM> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBM2005]
[FBM2005]	(Ferrari+Benoist+Maurogordato+, 2005)= ([FBM2005a])
Write:	<<[FBM2005] NNN>>
N:	239
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Optical photometry at the MPG/ESO 2.2m telescope at La Silla. Optical spectroscopy at the ESO 3.6m telescope. Identification of galaxies in ACO 392.
in source:	ACO 3921
Ref:	=2005A&A...430...19F
by	FERRARI C. , BENOIST C., MAUROGORDATO S., CAPPI A., SLEZAK E.
	Astron. Astrophys., 430, 19-38 (2005)
	Dynamical state and star formation properties of the merging galaxy cluster Abell 3921.
o	Table a: <[FBM2005] NNN> (Nos 1-239).
=E=	Catalogue in electronic form as J/A+A/430/19
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBM2005a]
[FBM2005a]	(Ferrari+Benoist+Maurogordato+, 2005)
*****	Avoid the usage of [FBM2005a], prefer [FBM2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBM2005b]
[FBM2005b]	(Firpo+Bosch+Morrell, 2005) (Not yet in Simbad)
Write:	<<[FBM2005b] NGC NNNN R>>
N:	2+2
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Search for giant HII regions in NGC 2997 and NGC 7552 at the 6.5m Magellan II Telescope, LCO.
in source:	NGC 2997
in source:	NGC 7552
Ref:	=2005MNRAS.356.1357F
by	FIRPO V. , BOSCH G., MORRELL N.
	Mon. Not. R. Astron. Soc., 356, 1357-1361 (2005)
	New giant HII regions in the southern sky.
o	Table 1, Figs 1, 2: <[FBM2005b] NGC 2997 R> (Nos I, II), <[FBM2005b] NGC 7552 R> (Nos I, IV).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBM2009]
[FBM2009]	(Farina+Bosch+Morrell+, 2009)= (Farina)
Write:	<<[FBM2009] NNN>>
N:	189
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Las Campanas 2.5m du Pont telescope spectroscopic observations of the N159/N160 complex.
in source:	Magellanic Clouds:LMC:LHA 120-N 159 = LHA 120-N 159
in source:	Magellanic Clouds:LMC:LHA 120-N 160 = LHA 120-N 160
Ref:	=2009AJ....138..510F
by	FARINA C. , BOSCH G.L., MORRELL N.I., BARBA R.H., WALBORN N.R.
	Astron. J., 138, 510-516 (2009)
	Spectroscopic study of the N159/N160 complex in the Large Magellanic Cloud.
o	Table 1: <[FBM2009] NNN> (Nos 1-189).
=E=	Catalogue in electronic form as <J/AJ/138/510/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBM2010]
[FBM2010]	(Fenech+Beswick+Muxlow+, 2010)
Write:	<<[FBM2010] xx.xx+yy.y>>
N:	36
Object:	(Rad) + SNR + HII (SIMBAD class: Radio = Radio Source)
Note:	MERLIN and VLBI observations at 1.7GHz of N=36 radio sources of the starburst galaxy M82. In the format: offset relative to RA = 09h51m, Dec = +69deg54' (1950). See also [MPW94], [MMW2002], [RVZ2004] and <%M [FMB2008].
in source:	M 82 = NGC 3034
Ref:	=2010MNRAS.408..607F
by	FENECH D. , BESWICK R., MUXLOW T.W.B., PEDLAR A., ARGO M.K.
	Mon. Not. R. Astron. Soc., 408, 607-621 (2010)
	Wide-field global VLBI and MERLIN combined monitoring of supernova remnants in M82.
o	Table 5: <[FBM2010] xx.xx+yy.y> N=36.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FBM82
FBM82	(Frogel+Blanco+McCarthy+, 1982)
*****	Avoid the usage of FBM82, prefer FBMC
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBM94]
[FBM94]	(Fabricant+Bautz+McClintock, 1994)
Write:	<<[FBM94] Cl 0303+1658 NNN>> <<[FBM94] Cl 0302+1717 NNN>>
N:	224+323
Object:	G + * in Cl (SIMBAD class: Unknown = Object of Unknown Nature)
in source:	ClG 0303+1658
in source:	ClG 0302+1717
Ref:	=1994AJ....107....8F
by	FABRICANT D.G. , BAUTZ M.W., McCLINTOCK J.E.
	Astron. J., 107, 8-23 (1994)
	Galaxy evolution in distant, X-ray selected clusters of galaxies. II. Cl 0303+1658 and Cl 0303+1717.
o	Misprint in the title: Cl 0302+1717 (not 0303)
o	Table 4: <[FBM94] Cl 0303+1658 NNN> N=224, Table 5: <[FBM94] Cl 0302+1717 NNN> N=323
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBM98]
[FBM98]	(Ferreras+Benitez+Martinez-Gonzalez, 1998) (Not yet in Simbad)
Write:	<<[FBM98] NN>>
N:	21
Object:	Poss. G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=21 candidates for high redshift late-type galaxies in the field around the QSO PC 1643+4631A.
Ref:	=1998A&A...333...43F
by	FERRERAS I. , BENITEZ N., MARTINEZ-GONZALEZ E.
	Astron. Astrophys., 333, 43-47 (1998)
	Imaging around PC 1643+4631A at the Lyman limit.
o	Table 3: [HR94] red objects
o	Table 2: <[FBM98] NN> (Nos 1-21)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FBMC
FBMC	(Frogel+Blanco+McCarthy+Cohen)= (BM) = (F) = ([FBM82])
Write:	<<FBMC Fornax NN>> <<FBMC Sculptor NN>>
N:	34+25
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 2: format 'Fornax NN', N=34 cool stars in the field of Fornax dw. G. Table 3: format 'Sculptor NN', N=25 cool stars in the field of Sculptor dw. G. Maps
in source:	NAME Fornax Dwarf Galaxy
in source:	NAME SDIG
Ref:	=1982ApJ...252..133F
by	FROGEL J.A. , BLANCO V.M., McCARTHY M.F., COHEN J.G.
	Astrophys. J., 252, 133-146 (1982)
	The late-type stellar content of the Fornax and Sculptor dwarf galaxies.
o	Table 2: <FBMC Fornax NN> (Nos 1-34). Table 3: <FBMC Sculptor NN> (Nos 1-25)
Origin	of the Acronym: L (1983ApJ...264..114R)
Details on Acronym: [FBN2016]
[FBN2016]	(Fabrizio+Bono+Nonino+, 2016)
Write:	<<[FBN2016] NNNNNN>>
N:	2748
Object:	* (SIMBAD class: Star)
Note:	VLT FLAMES (UVES and GIRAFFE), FORS2 and VIMOS spectroscopic observations of N=2748 stars in the field of the Carina dwarf spheroidal galaxy. Use of archival data from the Magellan/MMFS survey.
in source:	NAME Carina Dwarf Galaxy
Ref:	=2016ApJ...830..126F
by	FABRIZIO M. , BONO G., NONINO M., LOKAS E.L., FERRARO I., IANNICOLA G., BUONANNO R., CASSISI S., COPPOLA G., DALL'ORA M., GILMOZZI R., MARCONI M., MONELLI M., ROMANIELLO M., STETSON P.B., THEVENIN F., WALKER A.R.
	Astrophys. J., 830, 126-126 (2016)
	The Carina project. X. On the kinematics of old and intermediate-age stellar populations.
o	Table 2: <[FBN2016] NNNNNN> N=2748 among (Nos 3145-162379).
=E=	Catalogue in electronic form as J/ApJ/830/126
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBN87]
[FBN87]	(Fosbury+Bird+Nicholson+, 1987)
Write:	<<[FBN87] GN>>
N:	2
Object:	G in Pair (SIMBAD class: GinPair = Galaxy in Pair of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Identification of PKS 1934-63: N=2 galaxies in Pair, G1 is the brightest, it is the optical image of the PKS. G2 is the faintest component, west of G1. In 1986ApJ...311..526H, 2 components East and West are defined, now known as the 2 galaxies.
Ref:	=1987MNRAS.225..761F
by	FOSBURY R.A.E. , BIRD M.C., NICHOLSON W., WALL J.V.
	Mon. Not. R. Astron. Soc., 225, 761-768 (1987)
	The identification and nature of the powerful radio galaxy PKS 1934-63.
o	<[FBN87] GN> (Nos G1-G2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBP2004]
[FBP2004]	(Fabbiano+Baldi+Pellegrini+, 2004)
Write:	<<[FBP2004] SN>> <<[FBP2004] WW>>
N:	4+1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS observations of the nucleus of NGC 821.
in source:	NGC 821
Ref:	=2004ApJ...616..730F
by	FABBIANO G. , BALDI A., PELLEGRINI S., SIEMIGINOWSKA A., ELVIS M., ZEZAS A., McDOWELL J.
	Astrophys. J., 616, 730-737 (2004)
	Chandra observations of the quiescent nuclear black hole of NGC 821: evidence of nuclear activity.
o	Fig.2: <[FBP2004] AN> (Nos S1-S3), <[FBP2004] WW> (No. NE).
Ref:	=2007ApJ...667..731P
by	PELLEGRINI S. , BALDI A., KIM D.W., FABBIANO G., SORIA R., SIEMIGINOWSKA A., ELVIS M.
	Astrophys. J., 667, 731-748 (2007)
	A deep Chandra look at the low-L_{B} elliptical NGC 821: X-ray binaries, a galactic wind, and emission at the nucleus.
o	Table 5, Fig.7: <[FBP2004] SN> (No. S4) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBP2005]
[FBP2005]	(Foley+Bloom+Prochaska+, 2005)
Write:	<<[FBP2005] G1>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Note:	Keck II DEIMOS spectroscopy of GRB 051227.
Ref:	=2005GCN..4409....1F
by	FOLEY R.J. , BLOOM J.S., PROCHASKA J.X., ILLINGWORTH G.D., HOLDEN B.P., MAGEE D., CHALLIS P., GARG A.
	GRB Coordinates Network, Circular Service, 4409, 1-None (2005)
	GRB 051227: Keck spectroscopy.
o	<[FBP2005] G1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBP2008]
[FBP2008]	(Fox+Bergeron+Petitjean, 2008) (Not yet in Simbad)
Write:	<<[FBP2008] QSO JHHMM+DDMM abs N.NNNN>>
N:	35
Object:	Absorber
Note:	N=35 absorbers in 16 QSOs spectra.
Ref:	=2008MNRAS.388.1557F
by	FOX A.J. , BERGERON J., PETITJEAN P.
	Mon. Not. R. Astron. Soc., 388, 1557-1581 (2008)
	A study of quasar proximity in O VI absorbers at z = 2-3.
o	Table 1: <[FBP2008] QSO JHHMM+DDMM abs N.NNNN> N=35.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBP97]
[FBP97]	(Fernini+Burns+Perley, 1997)
Write:	<<[FBP97] 3C NNN.N A>>
N:	43
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	N=43 radio components in 8 radio galaxies from the 3CR catalogue. See also [FBB93]
Ref:	=1997AJ....114.2292F
by	FERNINI I. , BURNS J.O., PERLEY R.A.
	Astron. J., 114, 2292-2312 (1997)
	VLA imaging of Fanaroff-Riley II 3CR radio galaxies. II. Eight new images and comparisons with 3CR quasars.
o	in ref list: Garrington+ MNRAS.250.171 misprint for p. 271, Orr+ MNRAS.200 misprint for 100
o	Table 7: <[FBB93] 3C 55 F9> added. Fig.2: <[FBP97] 3C 20 A> (Nos A-E). Fig.5: <[FBP97] 3C 34 A> (Nos A-H). Fig.8: <[FBP97] 3C 42 A> (Nos A-D). Fig.10: <[FBP97] 3C 244.1 A> (Nos A-E). Fig.13: <[FBP97] 3C 252 A> (Nos A-E). Fig.16: <[FBP97] 3C 325 A> (Nos A-H). Fig.18-20: <[FBP97] 3C 330 A> (Nos A-F). Table 7: <[FBP97] 3C 22 A> (Nos A-B>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FBQS
FBQS	(FIRST Bright QSO Survey)= (BQ)
Write:	<<FBQS JHHMM+DDMM>>
N:	1318+264
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Note:	Faint Images of the Radio Sky at Twenty centimers (FIRST). Objects are QSO, with some G and *.
Ref:	=1996AJ....112..407G
by	GREGG M.D. , BECKER R.H., WHITE R.L., HELFAND D.J., McMAHON R.G., HOOK I.M.
	Astron. J., 112, 407-415 (1996)
	The FIRST bright QSO survey.
o	Tables 1 to 4: <FBQS JHHMM+DDMM> N=173
Ref:	=2000ApJS..126..133W
by	WHITE R.L. , BECKER R.H., GREGG M.D., LAURENT-MUEHLEISEN S.A., BROTHERTON M.S., IMPEY C.D., PETRY C.E., FOLTZ C.B., CHAFFEE F.H., RICHARDS G.T., OEGERLE W.R., HELFAND D.J., McMAHON R.G., CABANELA J.E.
	Astrophys. J., Suppl. Ser., 126, 133-207 (2000)
	The FIRST bright quasar survey. II. 60 nights and 1200 spectra later.
o	Tables 2 to 8: <FBQS JHHMM+DDMM> N=1318.
Ref:	=2001ApJS..135..227B
by	BECKER R.H. , WHITE R.L., GREGG M.D., LAURENT-MUEHLEISEN S.A., BROTHERTON M.S., IMPEY C.D., CHAFFEE F.H., RICHARDS G.T., HELFAND D.J., LACY M., COURBIN F., PROCTOR D.D.
	Astrophys. J., Suppl. Ser., 135, 227-262 (2001)
	The FIRST bright quasar survey. III. The South Galactic Cap.
o	Tables 1-7: <FBQS JHHMM+DDMM> N=264 new.
=E=	Catalogue in electronic form as J/AJ/112/407
=E=	Catalogue in electronic form as J/ApJS/126/133
=E=	Catalogue in electronic form as J/ApJS/135/227
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FBR2002]
[FBR2002]	(Filipovic+Bohlsen+Reid+, 2002)= (ATCA)
Write:	<<[FBR2002] JHHMMSS+DDMMSS>>
N:	718
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA study of the SMC.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2002MNRAS.335.1085F
by	FILIPOVIC M.D. , BOHLSEN T., REID W., STAVELEY-SMITH L., JONES P.A., NOHEJL K., GOLDSTEIN G.
	Mon. Not. R. Astron. Soc., 335, 1085-1090 (2002)
	An ATCA radio-continuum study of the Small Magellanic Cloud - I. Source catalogues at 1.42, 2.37, 4.80 and 8.64 GHz.
o	Tables 3-6: <[FBR2002] JHHMMSS+DDMMSS> N=718.
=E=	Catalogue in electronic form as J/MNRAS/335/1085
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBR2004]
[FBR2004]	(Fechner+Baade+Reimers, 2004)
Write:	<<[FBR2004] Absorber NN>>
N:	12
Object:	Absorber
Note:	Analysis of absorption features associated with HE 2347-4342.
Ref:	=2004A&A...418..857F
by	FECHNER C. , BAADE R., REIMERS D.
	Astron. Astrophys., 418, 857-867 (2004)
	The associated system of HE 2347-4342.
o	Table 2: <[FBR2004] Absorber NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FBS
FBS	(First Biurakan Survey)
Write:	<<FBS HHMM+DDdA>> <<FBS L NN-NNN>>
N:	25+?+30+20+18+42+31+79+123+169+88+57+161+118+72+1045+1471
Object:	Late * (SIMBAD class: Star)
Note:	'L' in the format stands for Late-type star, and the 1st digits 'NN' for the No. of the list (1 to 14). Each obj. have 2 formats 'FBS L NN-NNN' and 'FBS HHMM+DDd' or 'FBS HHMM+DDdA'. Identif. charts.
Ref:	=1989Afz....31..601A
by	ABRAHAMYAN G.V. , GIGOYAN K.S.
	Astrofizika, 31, 601-603 (1989)
	The first Byurakan spectral sky survey. Late-type stars. I. Zone +37 ° < del < +41 °.
o	<FBS HHMM+DDd> = <FBS L 1-NN> N=25
Ref:	=1990Afz....32..501A
by	ABRAHAMYAN G.V. , GIGOYAN K.S.
	Astrofizika, 32, 501-None (1990)
	First Byurakan spectroscopic sky survey. Late-type stars. II.
o	<FBS L 2-NN> = <FBS HHMM+DDd> N=25.
Ref:	=1990Afz....33..317A
by	ABRAHAMYAN G.V. , GIGOYAN K.S.
	Astrofizika, 33, 317-None (1990)
	The first Byurakan spectral survey - late type stars. III. Zone +33 δ +37.
o	<FBS HHMM+DDd> = <FBS L 3-NN> N=30
Ref:	=1993Afz....36..431A
by	ABRAMIAN G.V. , GIGHOIAN K.S.
	Astrofizika, 36, 431-433 (1993)
	First Byurakan spectroscopic sky survey. Late-type stars. IV. +61<δ<65 band.
o	<FBS HHMM+DDd> = <FBS L 4-NN> N=20
Ref:	=1994Ap.....37..322A
by	ABRAMYAN G.V. , GIGOYAN K.S.
	Astrophysics, 37, 322-325 (1994)
	The first Byurakan spectral sky survey. Stars of later spectral classes. V. The zone +65°.<δ<+69°.
o	<FBS HHMM+DDd> = <FBS L 5-NN> N=18
Ref:	=1995Ap.....38..115A
by	ABRAMYAN G.V. , GIGOYAN K.S.
	Astrophysics, 38, 115-118 (1995)
	The first Byurakan spectral sky survey. Late-type stars. VI. The zone +69 ° <δ< +77 °.
o	<FBS HHMM+DDd> = <FBS L 6-NN> (Nos 1-42)
Ref:	=1995Ap.....38..195A
by	ABRAMYAN G.V. , GIGOYAN K.S., SHAKHBAZYAN G.M.
	Astrophysics, 38, 195-199 (1995)
	The first Byurakan spectral sky survey. Late spectral class stars. VII. The zone +76 °<δ<+80 °.
o	<FBS HHMM+DDd> = <FBS L 7-NN> (Nos 1-31)
Ref:	=1996Ap.....39..310G
by	GIGOYAN K.S. , HAMBARYAN V.V.
	Astrophysics, 39, 310-314 (1996)
	First Byurakan Spectral Sky Survey. Late-type stars. VIII. Zone +80°.<δ <+90°.
o	Table 1: <FBS HHMM+DDd> = <FBS L 8-NN> (Nos 1-79)
Ref:	=1997Ap.....40..131A
by	ABRAHAMYAN H.V. , GIGOYAN K.S., HAMBARYAN V.V., AZZOPARDI M.
	Astrophysics, 40, 131-139 (1997)
	First Byurakan spectral sky survey. Stars of late spectral types. IX. -15 ° < δ < -11 ° belt.
o	Table 1: <FBS L 9-NNN> (Nos 1-123) = <FBS HHMM+DDdA>
Ref:	=1998Ap.....41..356G
by	GIGOYAN K.S. , HAMBARYAN V.V., AZZOPARDI M.
	Astrophysics, 41, 356-366 (1998)
	First Byurakan spectral sky survey. Stars of late spectral types. -11 ° < δ < -7 ° belt.
o	Positions and corss-identifications reviewed by Brian Skiff, in table1-a and notes-a
o	Table 1: <FBS L 10-NNN> (Nos 1-169) = <FBS HHMM+DDd> N=169.
Ref:	=2001Ap.....44...88G
by	GIGOYAN K.S. , ABRAHAMYAN H.V., AZZOPARDI M., RUSSEIL D.
	Astrophysics, 44, 88-97 (2001)
	First Byurakan spectral sky survey. Stars of late spectral types. XI. Zone -7° <δ < -3° .
o	Table 1, col(2): 083-049, 083-053, 093-056 (2000 coordinates) are respectively FBS 0838-049, FBS 0839-053, FBS 0934-056
o	Table 1: <FBS L 11-NN> (Nos 1-88) = <FBS HHMM+DDd>.
Ref:	=2001Ap.....44..328G
by	GIGOYAN K.S. , ABRAHAMYAN H.V., AZZOPARDI M., RUSSEIL D.
	Astrophysics, 44, 328-334 (2001)
	First Byurakan spectral sky survey. Stars of late spectral types. XII. Zone -3° < δ < +1° .
o	Table 1: <FBS L 12-NN> (Nos 1-57) = <FBS HHMM+DDd>.
Ref:	=2002Ap.....45..322G
by	GIGOYAN K.S. , ABRAHAMYAN H.V., AZZOPARDI M., RUSSEIL D.
	Astrophysics, 45, 322-333 (2002)
	First Byurakan Spectral Sky Survey types. XIII. Zone +1° ≤ δ ≤ +13°.
o	Table 1: <FBS L 13-NNN> (Nos 1-161) = <FBS HHMM+DDdA> N=161.
Ref:	=2003Ap.....46..475G
by	GIGOYAN K.S. , ABRAHAMYAN H.V., AZZOPARDI M., MAURON N., RUSSEIL D., SINAMYAN P.
	Astrophysics, 46, 475-488 (2003)
	First Byurakan Spectral Sky Survey. Stars of late-spectral types. XIV. Zone +13 ° ≤ δ ≤ +33 °.
o	Table 1: <FBS L 14-NNN> (Nos 1-118) = <FBS HHMM+DDdA> N=118.
Ref:	=2010Ap.....53..123G
by	GIGOYAN K.S. , SINAMYAN P.K., ENGELS D., MICKAELIAN A.M.
	Ap, 53, 123 (2010)
	First Byurakan Spectral Sky Survey. Stars of late spectral types. XV. Zone +45°≤δ≤+47°.
o	Table 1: <FBS L 15-NN> (Nos 1-72) = <FBS HHMM+DDd> N=72.
Ref:	=2012MNRAS.419.3346G
by	GIGOYAN K.S. , MICKAELIAN A.M.
	Mon. Not. R. Astron. Soc., 419, 3346-3353 (2012)
	Revised and updated catalogue of the first byurakan survey of late-type stars.
o	<FBS HHMM+DDdA> N=1045.
Ref:	=2019MNRAS.489.2030G
by	GIGOYAN K.S. , MICKAELIAN A.M., KOSTANDYAN G.R.
	Mon. Not. R. Astron. Soc., 489, 2030-2037 (2019)
	Revised and updated catalogue of the First Byurakan Survey of Late-Type Stars: second edition.
o	Table 1: <FBS HHMM+DDdA> N=1471.
=E=	Catalogue in electronic form as J/other/Ap/41.356
=E=	Catalogue in electronic form as J/other/Ap/44.88
=E=	Catalogue in electronic form as J/other/Ap/44.328
=E=	Catalogue in electronic form as J/other/Ap/45.322
=E=	Catalogue in electronic form as J/other/Ap/46.475
=E=	Catalogue in electronic form as III/246
=E=	Catalogue in electronic form as J/other/Ap/53.123
=E=	Catalogue in electronic form as III/266
=E=	Catalogue in electronic form as <J/MNRAS/489/2030/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FBS
FBS	(First Biurakan Survey)
Write:	<<FBS HHMM+DDd>> <<FBS B NNNN>>
N:	1103+143
Object:	* (SIMBAD class: Star)
Note:	'B' in the format for Blue star, EACH obj. have 2 formats 'FBS B NNNN' and 'FBS HHMM+DDd' from 1 to 1103. In the XIIth list, the numbering NNNN is not continued. Identif. charts.
Ref:	=1990Afz....32...29A
by	ABRAHAMIAN H.V. , LIPOVETSKY V.A., STEPANIAN J.A.
	Astrofizika, 32, 29-38 (1990)
	The First Byurakan Sky Survey. Blue stellar objects. I. Zone δ = +39.
o	FBS B 26 = FBS 0233+373, 0533 misprint. FBS B 99 :misprint in δ.
o	<FBS HHMM+DDd> = <FBS B NNN> (Nos 1-100)
Ref:	=1990Afz....33..213A
by	ABRAHAMIAN H.V. , LIPOVETSKY V.A., MICKAELIAN A.M., STEPANIAN J.A.
	Astrofizika, 33, 213-221 (1990)
	The first Byurakan spectral sky survey. Blue stellar objects. II. Zone Delta = +39°.
o	<FBS HHMM+DDd> = <FBS B NNN> (Nos 101-203)
Ref:	=1990Afz....33..345A
by	ABRAHAMIAN H.V. , LIPOVETSKY V.A., MICKAELIAN A.M., STEPANIAN D.A.
	Astrofizika, 33, 345-350 (1990)
	The first Byurakan spectral sky survey. Blue stellar objects. III. Zone δ =+ 43 °.
o	FBS B 283, misprint in δ : 56 instead of 54 ?, FBS B 312 : 1242+451 misprint for 1242+441.
o	<FBS HHMM+DDd> = <FBS B NNN> (Nos 204-323)
Ref:	=1991Afz....34...13A
by	ABRAMYAN G.V. , LIPOVETSKII V.A., MIKAELYAN A.M., STEPANYAN D.A.
	Astrofizika, 34, 13-20 (1991)
	First Byurakan spectral sky survey. Blue stellar objects. IV. The region +41<δ<45.
o	<FBS HHMM+DDd> = <FBS B NNN> (Nos 324-429)
Ref:	=1993Afz....36..109A
by	ABRAMYAN G.V. , MIKAELYAN A.M.
	Astrofizika, 36, 109-115 (1993)
	First Byurakan spectral sky survey. Blue stellar objects. V.
o	<FBS HHMM+DDd> = <FBS B NNN> (Nos 430-540)
Ref:	=1993Afz....36..517A
by	ABRAHAMIAN H.V. , MICKAELIAN A.M.
	Astrofizika, 36, 517-526 (1993)
	First Byurakan spectral sky survey. Blue stellar objects. VI. Zone +33 <δ< +37.
o	<FBS HHMM+DDd> = <FBS B NNN> (Nos 541-638)
Ref:	=1994Afz....37...43A
by	ABRAHAMIAN H.V. , MICKAELIAN A.M.
	Astrofizika, 37, 43-55 (1994)
	First Byurakan Spectral Sky Survey. Blue stellar objects. VII. Zone +61 <δ< +65.
o	<FBS HHMM+DDd> = <FBS B NNN> (Nos 639-757)
Ref:	=1994Afz....37..197A
by	ABRAHAMIAN H.V. , MICKAELIAN A.M.
	Astrofizika, 37, 197-206 (1994)
	First Byurakan Spectral Sky Survey. Blue stellar objects. VIII. Zone +65 °. < δ < +69 °.
o	<FBS B NNN> = <FBS HHMM+HHd> N=98, (Nos 758-855)
Ref:	=1994Ap.....37..224A
by	ABRAMYAN G.V. , MIKAELYAN A.M.
	Astrophysics, 37, 224-230 (1994)
	The first Byurakan spectral sky survey. Blue stellar objects. IX. The zone +69 ° <δ < +73 ° and additional objects from previous regions.
o	<FBS B NNN> = <FBS HHMM+HHd> N=84, (Nos 856-939)
Ref:	=1995Ap.....38..108A
by	ABRAMYAN G.V. , MIKAELYAN A.M.
	Astrophysics, 38, 108-114 (1995)
	The first Byurakan spectral sky survey. Blue stellar objects. X. The zone +73 ° < δ < +80 °.
o	<FBS B NNNN> = <FBS HHMM+HHd> N=100, (Nos 940-1039)
Ref:	=1996Ap.....39..315A
by	ABRAHAMIAN H.V. , MICKAELIAN A.M.
	Astrophysics, 39, 315-320 (1996)
	First Byurakan Spectral Sky Survey. Blue stellar objects. XI. Region +80°.<δ<+90°.
o	Table 2: <FBS HHMM+DDd> = <FBS B NNNN> (Nos 1040-1103>
Ref:	=2003Ap.....46...46A
by	ABRAHAMYAN G.V. , SINAMYAN P.K., GIGOYAN K.S.
	Astrophysics, 46, 46-57 (2003)
	First Byurakan Spectral Sky Survey. Blue stellar objects. XII. The region -3°.<δ<+1°.
o	Table 1 scannee par James Marcout : sequence numbering in column 1 no t used in SIMBAD, not continuing the 'FBS B NNNN' numbering.
o	Table 1: <FBS HHMM+DDd> N=143.
Ref:	=2008AJ....136..946M
by	MICKAELIAN A.M.
	Astron. J., 136, 946-953 (2008)
	Revised and updated catalogue of the First Byurakan Survey blue stellar objects.
o	Catalog: <FBS B NNNN> (Nos 1-1103) = <FBS HHMM+DDd> N=1103.
=E=	Catalogue in electronic form as II/223
=E=	Catalogue in electronic form as III/258
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FBS
FBS	(First Biurakan Survey)
Write:	<<FBS HHMM+DDdA>> <<FBS L NN-NNN>>
N:	25+?+30+20+18+42+31+79+123+169+88+57+161+118+72+1045+1471
Object:	Late * (SIMBAD class: Star)
Note:	'L' in the format stands for Late-type star, and the 1st digits 'NN' for the No. of the list (1 to 14). Each obj. have 2 formats 'FBS L NN-NNN' and 'FBS HHMM+DDd' or 'FBS HHMM+DDdA'. Identif. charts.
Ref:	=1989Afz....31..601A
by	ABRAHAMYAN G.V. , GIGOYAN K.S.
	Astrofizika, 31, 601-603 (1989)
	The first Byurakan spectral sky survey. Late-type stars. I. Zone +37 ° < del < +41 °.
o	<FBS HHMM+DDd> = <FBS L 1-NN> N=25
Ref:	=1990Afz....32..501A
by	ABRAHAMYAN G.V. , GIGOYAN K.S.
	Astrofizika, 32, 501-None (1990)
	First Byurakan spectroscopic sky survey. Late-type stars. II.
o	<FBS L 2-NN> = <FBS HHMM+DDd> N=25.
Ref:	=1990Afz....33..317A
by	ABRAHAMYAN G.V. , GIGOYAN K.S.
	Astrofizika, 33, 317-None (1990)
	The first Byurakan spectral survey - late type stars. III. Zone +33 δ +37.
o	<FBS HHMM+DDd> = <FBS L 3-NN> N=30
Ref:	=1993Afz....36..431A
by	ABRAMIAN G.V. , GIGHOIAN K.S.
	Astrofizika, 36, 431-433 (1993)
	First Byurakan spectroscopic sky survey. Late-type stars. IV. +61<δ<65 band.
o	<FBS HHMM+DDd> = <FBS L 4-NN> N=20
Ref:	=1994Ap.....37..322A
by	ABRAMYAN G.V. , GIGOYAN K.S.
	Astrophysics, 37, 322-325 (1994)
	The first Byurakan spectral sky survey. Stars of later spectral classes. V. The zone +65°.<δ<+69°.
o	<FBS HHMM+DDd> = <FBS L 5-NN> N=18
Ref:	=1995Ap.....38..115A
by	ABRAMYAN G.V. , GIGOYAN K.S.
	Astrophysics, 38, 115-118 (1995)
	The first Byurakan spectral sky survey. Late-type stars. VI. The zone +69 ° <δ< +77 °.
o	<FBS HHMM+DDd> = <FBS L 6-NN> (Nos 1-42)
Ref:	=1995Ap.....38..195A
by	ABRAMYAN G.V. , GIGOYAN K.S., SHAKHBAZYAN G.M.
	Astrophysics, 38, 195-199 (1995)
	The first Byurakan spectral sky survey. Late spectral class stars. VII. The zone +76 °<δ<+80 °.
o	<FBS HHMM+DDd> = <FBS L 7-NN> (Nos 1-31)
Ref:	=1996Ap.....39..310G
by	GIGOYAN K.S. , HAMBARYAN V.V.
	Astrophysics, 39, 310-314 (1996)
	First Byurakan Spectral Sky Survey. Late-type stars. VIII. Zone +80°.<δ <+90°.
o	Table 1: <FBS HHMM+DDd> = <FBS L 8-NN> (Nos 1-79)
Ref:	=1997Ap.....40..131A
by	ABRAHAMYAN H.V. , GIGOYAN K.S., HAMBARYAN V.V., AZZOPARDI M.
	Astrophysics, 40, 131-139 (1997)
	First Byurakan spectral sky survey. Stars of late spectral types. IX. -15 ° < δ < -11 ° belt.
o	Table 1: <FBS L 9-NNN> (Nos 1-123) = <FBS HHMM+DDdA>
Ref:	=1998Ap.....41..356G
by	GIGOYAN K.S. , HAMBARYAN V.V., AZZOPARDI M.
	Astrophysics, 41, 356-366 (1998)
	First Byurakan spectral sky survey. Stars of late spectral types. -11 ° < δ < -7 ° belt.
o	Positions and corss-identifications reviewed by Brian Skiff, in table1-a and notes-a
o	Table 1: <FBS L 10-NNN> (Nos 1-169) = <FBS HHMM+DDd> N=169.
Ref:	=2001Ap.....44...88G
by	GIGOYAN K.S. , ABRAHAMYAN H.V., AZZOPARDI M., RUSSEIL D.
	Astrophysics, 44, 88-97 (2001)
	First Byurakan spectral sky survey. Stars of late spectral types. XI. Zone -7° <δ < -3° .
o	Table 1, col(2): 083-049, 083-053, 093-056 (2000 coordinates) are respectively FBS 0838-049, FBS 0839-053, FBS 0934-056
o	Table 1: <FBS L 11-NN> (Nos 1-88) = <FBS HHMM+DDd>.
Ref:	=2001Ap.....44..328G
by	GIGOYAN K.S. , ABRAHAMYAN H.V., AZZOPARDI M., RUSSEIL D.
	Astrophysics, 44, 328-334 (2001)
	First Byurakan spectral sky survey. Stars of late spectral types. XII. Zone -3° < δ < +1° .
o	Table 1: <FBS L 12-NN> (Nos 1-57) = <FBS HHMM+DDd>.
Ref:	=2002Ap.....45..322G
by	GIGOYAN K.S. , ABRAHAMYAN H.V., AZZOPARDI M., RUSSEIL D.
	Astrophysics, 45, 322-333 (2002)
	First Byurakan Spectral Sky Survey types. XIII. Zone +1° ≤ δ ≤ +13°.
o	Table 1: <FBS L 13-NNN> (Nos 1-161) = <FBS HHMM+DDdA> N=161.
Ref:	=2003Ap.....46..475G
by	GIGOYAN K.S. , ABRAHAMYAN H.V., AZZOPARDI M., MAURON N., RUSSEIL D., SINAMYAN P.
	Astrophysics, 46, 475-488 (2003)
	First Byurakan Spectral Sky Survey. Stars of late-spectral types. XIV. Zone +13 ° ≤ δ ≤ +33 °.
o	Table 1: <FBS L 14-NNN> (Nos 1-118) = <FBS HHMM+DDdA> N=118.
Ref:	=2010Ap.....53..123G
by	GIGOYAN K.S. , SINAMYAN P.K., ENGELS D., MICKAELIAN A.M.
	Ap, 53, 123 (2010)
	First Byurakan Spectral Sky Survey. Stars of late spectral types. XV. Zone +45°≤δ≤+47°.
o	Table 1: <FBS L 15-NN> (Nos 1-72) = <FBS HHMM+DDd> N=72.
Ref:	=2012MNRAS.419.3346G
by	GIGOYAN K.S. , MICKAELIAN A.M.
	Mon. Not. R. Astron. Soc., 419, 3346-3353 (2012)
	Revised and updated catalogue of the first byurakan survey of late-type stars.
o	<FBS HHMM+DDdA> N=1045.
Ref:	=2019MNRAS.489.2030G
by	GIGOYAN K.S. , MICKAELIAN A.M., KOSTANDYAN G.R.
	Mon. Not. R. Astron. Soc., 489, 2030-2037 (2019)
	Revised and updated catalogue of the First Byurakan Survey of Late-Type Stars: second edition.
o	Table 1: <FBS HHMM+DDdA> N=1471.
=E=	Catalogue in electronic form as J/other/Ap/41.356
=E=	Catalogue in electronic form as J/other/Ap/44.88
=E=	Catalogue in electronic form as J/other/Ap/44.328
=E=	Catalogue in electronic form as J/other/Ap/45.322
=E=	Catalogue in electronic form as J/other/Ap/46.475
=E=	Catalogue in electronic form as III/246
=E=	Catalogue in electronic form as J/other/Ap/53.123
=E=	Catalogue in electronic form as III/266
=E=	Catalogue in electronic form as <J/MNRAS/489/2030/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FBS2006]
[FBS2006]	(Feretti+Bacchi+Slee+, 2006)= ([FBS2006a])
Write:	<<[FBS2006] A>> <<[FBS2006] NNa>>
N:	3+15
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA and ATCA observations of 3 diffuse and 12 discrete radio sources in the field of ACO 548.
in source:	ACO 548
Ref:	=2006MNRAS.368..544F
by	FERETTI L. , BACCHI M., SLEE O.B., GIOVANNINI G., GOVONI F., ANDERNACH H., TSAREVSKY G.
	Mon. Not. R. Astron. Soc., 368, 544-552 (2006)
	Diffuse radio sources in the cluster of galaxies Abell 548b.
o	Fig.1, Table 2: <[FBS2006] A> (Nos A-C). Table 3: <[FBS2006] NNa> (Nos 1-12, 7a-7c).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBS2006a]
[FBS2006a]	(Feretti+Bacchi+Slee+, 2006)
*****	Avoid the usage of [FBS2006a], prefer [FBS2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBS2006b]
[FBS2006b]	(Fish+Brisken+Sjouwerman+, 2006) (Not yet in Simbad)
Write:	<<[FBS2006b] NNN>>
N:	253
Object:	OH Maser Spot (SIMBAD class: Maser)
Note:	VLBA observations of hydroxyl masers in W3(OH).
in source:	W 3:W 3(OH) = W 3(OH)
Ref:	=2006ApJ...647..418F
by	FISH V.L. , BRISKEN W.F., SJOUWERMAN L.O.
	Astrophys. J., 647, 418-431 (2006)
	A very high spectral resolution study of ground-state OH masers in W3(OH).
o	Table 1: <[FBS2006b] NNN> (Nos 1-253).
=E=	Catalogue in electronic form as J/ApJ/647/418
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBS2011]
[FBS2011]	(Fassbender+Boehringer+Santos+, 2011)
Write:	<<[FBS2011] NN>>
N:	13
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 and LBT LBC observations of the galaxy cluster XMMU J1230.3+1339.
in source:	NAME XMMU J12303+1339
Ref:	=2011A&A...527A..78F
by	FASSBENDER R. , BOEHRINGER H., SANTOS J.S., PRATT G.W., SUHADA R., KOHNERT J., LERCHSTER M., ROVILOS E., PIERINI D., CHON G., SCHWOPE A.D., LAMER G., MUEHLEGGER M., ROSATI P., QUINTANA H., NASTASI A., DE HOON A., SEITZ S., MOHR J.J.
	Astron. Astrophys., 527A, 78-78 (2011)
	A pan-chromatic view of the galaxy cluster XMMU J1230.3+1339 at z = 0.975. Observing the assembly of a massive system.
o	Table 2: <[FBS2011] NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBS2016]
[FBS2016]	(Figuera Jaimes+Bramich+Skottfelt+, 2016)
Write:	<<[FBS2016] NGC104 EMN>>
N:	7
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	ESO Danish 1.54m telescope EMCCD observations of N=7 variable stars in the Galactic globular cluster NGC 104.
in source:	NGC 104
Ref:	=2016A&A...588A.128F
by	FIGUERA JAIMES R. , BRAMICH D.M., SKOTTFELT J., KAINS N., JORGENSEN U.G., HORNE K., DOMINIK M., ALSUBAI K.A., BOZZA V., CALCHI NOVATI S., CICERI S., D'AGO G., GALIANNI P., GU S.-H., HARPSOE K.B.W., HAUGBOLLE T., HINSE T.C., HUNDERTMARK M., JUNCHER D., KORHONEN H., MANCINI L., POPOVAS A., RABUS M., RAHVAR S., SCARPETTA G., SCHMIDT R.W., SNODGRASS C., SOUTHWORTH J., STARKEY D., STREET R.A., SURDEJ J., WANG X.-B., WERTZ O.
	Astron. Astrophys., 588A, 128-128 (2016)
	Exploring the crowded central region of ten Galactic globular clusters using EMCCDs.
o	Paragraph 8.4.1: V11 probably Cl* NGC 6093 DN 1. Paragraph 8.5: V81 = [KTR2013] V58 = Cl* NGC 6121 SAW V81 and V101 = [NBH2014] 3487 = Cl* NGC 6121 SAW V101. For objects Cl* NGC 5286 SAW V37 to V58, there is a ~6 arcsec difference between coordinates from 2016A&A...588A.128F and coordinates from 2010AJ....139..357Z.
o	Table 4: <[FBS2016] NGC104 EMN> N=7 (Nos EM1-EM7). Table 5: <Cl* NGC 5139 SAW VNNN> N=3 (Nos V457-V459) added. Table 6: <Cl* NGC 5286 SAW VNN> N=11 (Nos V63-V73) added, Table 7: <Cl* NGC 6093 SAW VNN> N=7 (Nos V34-V40) added. Table 9: <Cl* NGC 6541 SAW VNN> N=2 (Nos V21-V22) added, Table 11: <Cl* NGC 6681 SAW VN> N=1 (No V6) added.
=E=	Catalogue in electronic form as J/A+A/588/A128
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBS82]
[FBS82]	(Fosbury+Boksenberg+Snijders+, 1982)
Write:	<<[FBS82] A>>
N:	4
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=4 galaxies in group in the field of PKS 2158-380 (galaxy A).
Ref:	=1982MNRAS.201..991F
by	FOSBURY R.A.E. , BOKSENBERG A., SNIJDERS M.A.J., DANZIGER I.J., DISNEY M.J., GOSS W.M., PENSTON M.V., WAMSTEKER W., WELLINGTON K.J., WILSON A.S.
	Mon. Not. R. Astron. Soc., 201, 991-1008 (1982)
	Very extended ionized gas in radio galaxies- I. A radio, optical and ultraviolet study of PKS 2158-380.
o	Plate 2(b): <[FBS82] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FBW
FBW	(Fornax dwarf galaxy, Bersier+Wood)
Write:	<<FBW JHHMMSS.s+DDMMSS>>
N:	618
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	Search for variable stars in the Fornax dwarf galaxy. 0.5 square degree covered. Data in V and I bands. T.2: N=513 RR Lyr., T.3: N=25 Cepheids, T.4: N=85 LPV candidates.
in source:	NAME Fornax Dwarf Galaxy
Ref:	=2002AJ....123..840B
by	BERSIER D. , WOOD P.R.
	Astron. J., 123, 840-847 (2002)
	Variable stars in the Fornax dwarf galaxy.
o	Tables 2, 3, 4: <FBW JHHMMSS.s+DDMMSS> N=618.
=E=	Catalogue in electronic form as J/AJ/123/840
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [FBZ2007]
[FBZ2007]	(Fathi+Beckman+Zurita+, 2007)
Write:	<<[FBZ2007] NNN>>
N:	376
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Halpha Fabry-Perot observations of NGC 628 at the 1.6m telescope at the Observatoire du Mont Megantic, Canada.
in source:	NGC 628 = M 74
Ref:	=2007A&A...466..905F
by	FATHI K. , BECKMAN J.E., ZURITA A., RELANO M., KNAPEN J.H., DAIGLE O., HERNANDEZ O., CARIGNAN C.
	Astron. Astrophys., 466, 905-916 (2007)
	Evolution of structure in late-type spiral galaxies. I. Ionized gas kinematics in NGC 628.
o	Table: <[FBZ2007] NNN> (Nos 1-376).
=E=	Catalogue in electronic form as J/A+A/466/905
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FBZ2009]
[FBZ2009]	(Fritz+Bohm+Ziegler, 2009)
Write:	<<[FBZ2009] WHDF-NNNa>>
N:	11
Object:	G (SIMBAD class: Galaxy)
Note:	VLT spectroscopy and HST/ACS photometry of early-type galaxies in the FORS Deep Field (FDF) and the William Herschel Deep Field (WHDF).
Ref:	=2009MNRAS.393.1467F
by	FRITZ A. , BOHM A., ZIEGLER B.L.
	Mon. Not. R. Astron. Soc., 393, 1467-1492 (2009)
	The evolution of field early-type galaxies in the FDF and WHDF.
o	Tables 4-5: <[FBZ2009] WHDF-NNNa> N=11 among (Nos 92-946).
=E=	Catalogue in electronic form as J/MNRAS/393/1467
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FC
FC	(Finding Chart)
*****	Avoid the usage of FC, prefer AG82
Details on Acronym: [FC2000]
[FC2000]	(Forster+Caswell, 2000)
Write:	<<[FC2000] GLLL.ll+B.bb A>>
N:	29
Object:	UC HII (SIMBAD class: HIIReg = HII Region)
Note:	Table 1: Peak positions of Ultra Compact HII in GPSR5 source regions. 'G9.62+0.20 E' is an OH maser.
Ref:	=2000ApJ...530..371F
by	FORSTER J.R. , CASWELL J.L.
	Astrophys. J., 530, 371-386 (2000)
	Radio continuum emission at OH and H_{2}O maser sites.
o	Table 1: <[FC2000] GLLL.ll+B.bb A> N=29.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FC2004]
[FC2004]	(Filliatre+Chaty, 2004)
Write:	<<[FC2004] Star N>>
N:	3
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	NTT ESO observations, using EMMI and SOFI instruments. Search for the optical counterpart of IGR J16318-4848: 3 stars are candidate counterparts, authors consider Star 1 as the counterpart.
Ref:	=2004ApJ...616..469F
by	FILLIATRE P. , CHATY S.
	Astrophys. J., 616, 469-484 (2004)
	The Optical/Near-infrared counterpart of the INTEGRAL obscured source IGR J16318-4848: an sgB[e] in a high-mass X-ray binary?
o	Fig.2, Table 2: <[FC2004] Star N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FC85]
[FC85]	(Flatters+Conway, 1985)
Write:	<<[FC85] N>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	[FC85] 1, 2, 3 = [BKS95] H1, 2, 3 repectively
in source:	3C 273
Ref:	=1985Natur.314..425F
by	FLATTERS C. , CONWAY R.G.
	Nature, 314, 425-426 (1985)
	The radio jet of the quasar 3C 273.
o	Table 1: the 3 components have been named later '[BKS95] HN' (Nos H1-H3)
o	<[FC85] N> (Nos 1-3)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FC98]
[FC98]	(Fassnacht+Cohen, 1998)
Write:	<<[FC98] BHHMM+DDd>> <<[FC98] BHHMM+DDd A>> <<[FC98] BHHMM+DDd G>> <<[FC98] BHHMM+DDd BS>>
N:	3+4+3+3
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=3 gravitational lens systems, 'B0712+472', 'B1030+074', and 'B1600+434'. Each system shows a lensing galaxy 'G' and a background source 'BS'. The two last systems shows two radio-components A and B. For [FC98] B1600+434, see also [JH97]. For [FC98] B0712+472, see also [JNB98]
in source:	CLASS B0712+472
in source:	CLASS B1030+074
in source:	CLASS B1600+434
Ref:	=1998AJ....115..377F
by	FASSNACHT C.D. , COHEN J.G.
	Astron. J., 115, 377-382 (1998)
	Keck spectroscopy of three gravitational lens systems discovered in the JVAS and CLASS surveys.
o	<[FC98] BHHMM+DDd> N=3, <[FC98] BHHMM+DDd A> N=4, <[FC98] BHHMM+DDd G> N=3, <[FC98] BHHMM+DDd BS> N=3
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCB2005]
[FCB2005]	(Foley+Chen+Bloom+, 2005)
Write:	<<[FCB2005] Host G>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Gemini-North GMOS search for the host galaxy of GRB 050525a.
Ref:	=2005GCN..3483....1F
by	FOLEY R.J. , CHEN H.-W., BLOOM J., PROCHASKA J.X.
	GRB Coordinates Network, Circular Service, 3483, 1-None (2005)
	GRB 050525a: Gemini/GMOS spectra.
o	<[FCB2005] Host G> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCB2007]
[FCB2007]	(Frye+Coe+Bowen+, 2007)
Write:	<<[FCB2007] JHHMMSS.sss+DDMMSS.ss>>
N:	15+91
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck LRIS, VLT FORS2, and Magellan LDSS-2 spectroscopy observations of ACO 1689.
in source:	ACO 1689
Ref:	=2007ApJ...665..921F
by	FRYE B.L. , COE D., BOWEN D.V., BENITEZ N., BROADHURST T., GUHATHAKURTA P., ILLINGWORTH G., MENANTEAU F., SHARON K., LUPTON R., MEYLAN G., ZEKSER K., MEURER G., HURLEY M.
	Astrophys. J., 665, 921-935 (2007)
	The Sextet Arcs: a strongly lensed Lyman break galaxy in the ACS spectroscopic galaxy survey toward Abell 1689.
o	The Sextet Arcs = NAME ACO 1689 SEXTET ARCS in SIMBAD.
o	Tables 1, 3: <[FCB2007] JHHMMSS.sss+DDMMSS.ss> N=15+91.
=E=	Catalogue in electronic form as J/ApJ/665/921
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCB2008]
[FCB2008]	(Fontani+Caselli+Bourke+, 2008)
Write:	<<[FCB2008] W>> <<[FCB2008] CN>> <<[FCB2008] CN-a>>
N:	2+4+2
Object:	Cloud + Condensation (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	SMA N2D+ and PdBI N2H+ observations of the star-forming region IRAS 05345+3157.
in source:	IRAS 05345+3157
Ref:	=2008A&A...477L..45F
by	FONTANI F. , CASELLI P., BOURKE T.L., CESARONI R., BRAND J.
	Astron. Astrophys., 477L, 45-48 (2008)
	Highly deuterated pre-stellar cores in a high-mass star formation region.
o	Figs 1, 2: <[FCB2008] W> (Nos N, S), <[FCB2008] CN> (Nos C1-C4).
Ref:	=2009A&A...499..233F
by	FONTANI F. , ZHANG Q., CASELLI P., BOURKE T.L.
	Astron. Astrophys., 499, 233-247 (2009)
	Linking pre- and proto-stellar objects in the intermediate-/high-mass star forming region IRAS 05345+3157.
o	Fig. 2, Table 3: <[FCB2008] CN-a> (Nos C1-a, C1-b).
=E=	Catalogue in electronic form as <J/A+A/499/233/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCB2017]
[FCB2017]	(Foex+Chon+Bohringer, 2017)
Write:	<<[FCB2017] JHHMMSS.s+DDMMSS.s>>
N:	4104
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT VIMOS spectroscopic and ESO/MPG 2.2m telescope WFI photometric observations of N=4104 galaxies in three galaxy clusters.
in source:	RXC J0225.9-4154
in source:	RXC J0528.9-3927
in source:	RXC J2308.3-0211
Ref:	=2017A&A...601A.145F
by	FOEX G. , CHON G., BOHRINGER H.
	Astron. Astrophys., 601A, 145-145 (2017)
	From the core to the outskirts: structure analysis of three massive galaxy clusters.
o	Table A.1: <[FCB2017] JHHMMSS.s+DDMMSS.s> N=4104.
o	Substructures not in SIMBAD.
=E=	Catalogue in electronic form as J/A+A/601/A145
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCB2020]
[FCB2020]	(Fang+Charles+Blandford, 2020)
Write:	<<[FCB2020] J1913+0515>>
N:	1
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	N=1 gamma-ray residual excess near FL8Y J1913.3+0515 in the field of the microquasar SS 433. Use of Fermi LAT data.
Ref:	=2020ApJ...889L...5F
by	FANG K. , CHARLES E., BLANDFORD R.D.
	Astrophys. J., 889L, 5-5 (2020)
	GeV-TeV counterparts of SS 433/W50 from Fermi-LAT and HAWC observations.
o	<[FCB2020] J1913+0515> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FCC
FCC	(Fornax Cluster Catalog)= (FCCB)
Write:	<<FCC NNN>> <<FCC BNNNN>>
N:	340+2338
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table II: G classified as cluster members and likely cluster members. Table III: 'B' in the format means Background. G classified as possible members and likely background galaxies.
in source:	NAME Fornax Cluster
Ref:	=1989AJ.....98..367F
by	FERGUSON H.C.
	Astron. J., 98, 367-418 (1989)
	Population studies in groups and clusters of galaxies. II. A catalog of galaxies in the central 3.5 °. of the Fornax cluster.
o	Table II: <FCC NNN> (Nos 1-340). Table III: <FCC BNNNN> (Nos B1-B2338)
=E=	Catalogue in electronic form as VII/180
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FCC2002]
[FCC2002]	(Furuya+Cesaroni+Codella+, 2002)
Write:	<<[FCC2002] ANa>>
N:	4+2+3
Object:	* (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	N=4 stars in the field of the star-forming region GAL 024.78+00.08. 2004ApJ...601L.187B: Star A is resolved in two separate cores. 2011A&A...532A..91B: Cores A1 and A2 are resolved into three and two cores respectively.
Ref:	=2002A&A...390L...1F
by	FURUYA R.S. , CESARONI R., CODELLA C., TESTI L., BACHILLER R., TAFALLA M.
	Astron. Astrophys., 390, 1-4 (2002)
	G24.78+0.08: A cluster of high-mass (proto)stars.
o	Fig.1, Table 1: <[FCC2002] A> (Nos A-D).
Ref:	=2004ApJ...601L.187B
by	BELTRAN M.T. , CESARONI R., NERI R., CODELLA C., FURUYA R.S., TESTI L., OLMI L.
	Astrophys. J., 601, 187-190 (2004)
	Rotating disks in high-mass young stellar objects.
o	Fig.1: <[FCC2002] AN> (Nos A1-A2) added.
Ref:	=2011A&A...532A..91B
by	BELTRAN M.T. , CESARONI R., ZHANG Q., GALVAN-MADRID R., BEUTHER H., FALLSCHEER C., NERI R., CODELLA C.
	Astron. Astrophys., 532A, 91-91 (2011)
	Molecular outflows and hot molecular cores in G24.78+0.08 at sub-arcsecond angular resolution.
o	Fig. 1, Table 2: <[FCC2002] ANa> (Nos A1b-A1c, A2b) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCC2008]
[FCC2008]	(Fiorentino Clementini Contrera+, 2008) (Not yet in Simbad)
Write:	<<[FCC2008] NNNNN>>
N:	4
Object:	Poss. Cepheid (SIMBAD class: Star)
Note:	N=4 Cepheid candidates in Zw I 18.
in source:	Zw I 18 = Mrk 116
Ref:	=2008MmSAI..79..461F
by	FIORENTINO G. , CLEMENTINI G., CONTRERAS R., MARCONI M., MUSELLA I., TOSI M., ALOISI A., ANNIBALI F., SAHA A.
	MmSAI, 79, 461-465 (2008)
	Very metal poor classical Cepheids: the distance of IZw18.
o	Table 1: <[FCC2008] NNNNN> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCC2010]
[FCC2010]	(Fiorentino+Contreras Ramos+Clementini+, 2010)
Write:	<<[FCC2010] VNN>>
N:	34
Object:	Poss. V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations of N=34 candidate variable stars in Zw I 18.
in source:	Zw I 18 = Mrk 116
Ref:	=2010ApJ...711..808F
by	FIORENTINO G. , CONTRERAS RAMOS R., CLEMENTINI G., MARCONI M., MUSELLA I., ALOISI A., ANNIBALI F., SAHA A., TOSI M., VAN DER MAREL R.P.
	Astrophys. J., 711, 808-817 (2010)
	Multi-epoch Hubble space telescope observations of IZw18: characterization of variable stars at ultra-low metallicities.
o	Tables 2-3: <[FCC2010] VNN> (Nos V1-V34).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCC2013]
[FCC2013]	(Fruth+Cabrera+Chini+, 2013)= (BEST II)
Write:	<<[FCC2013] FFF NNNNNN>>
N:	17+3083
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Berlin Exoplanet Search Telescope II (BEST II) observations of variable stars in three target fields.
Ref:	=2013AJ....146..136F
by	FRUTH T. , CABRERA J., CHINI R., CSIZMADIA Sz., DREYER C., EIGMULLER P., ERIKSON A., KABATH P., KIRSTE S., LEMKE R., MURPHY M., PASTERNACKI T., RAUER H., TITZ-WEIDER R.
	Astron. J., 146, 136 (2013)
	The Berlin Exoplanet Search Telescope II catalog of variable stars. I. Characterization of three southern target fields.
o	Tables 4-5: <[FCC2013] FFF NNNNNN> N=3083 among (Nos F17 00273 to F17 68159, F18 00214 to F18 10917, F19 000002 to F19 127586).
=E=	Catalogue in electronic form as <J/AJ/146/136/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCC99]
[FCC99]	(Filippenko+Chornock+Coil+, 1999)
Write:	<<[FCC99] JHHMMSS.s+DDMMSS>>
N:	1
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Stat:	is completely incorporated in Simbad
Note:	KAIT observations. Discovery of a new nova in M 31.
in source:	M 31 = NGC 224
Ref:	=1999IAUC.7272R...1F
by	FILIPPENKO A.V. , CHORNOCK R.T., COIL A.L., LEONARD D.C., LI W.D.
	IAU Circ., 7272, 1-None (1999)
	Novae in M 31.
o	<[FCC99] JHHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FCCB
FCCB	(Fornax Cluster Catalog, Background)
*****	Avoid the usage of FCCB, prefer FCC
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [FCD2016]
[FCD2016]	(Fumagalli+Cantalupo+Dekel+, 2016)
Write:	<<[FCD2016] NN>>
N:	91
Object:	Unknown (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT MUSE spectroscopic observations of N=91 galaxies in the proximity of two very metal-poor gas clouds at z∼3 towards the quasar Q0956+122.
Ref:	=2016MNRAS.462.1978F
by	FUMAGALLI M. , CANTALUPO S., DEKEL A., MORRIS S.L., O'MEARA J.M., PROCHASKA J.X., THEUNS T.
	Mon. Not. R. Astron. Soc., 462, 1978-1988 (2016)
	MUSE searches for galaxies near very metal-poor gas clouds at z ~ 3: new constraints for cold accretion models.
o	Table 2: <[FCD2016] NN> (Nos 1-91).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCE2001]
[FCE2001]	(Fabian+Crawford+Ettori+, 2001)
Write:	<<[FCE2001] JHHMMSS.sss+DDMMSS.ss>>
N:	1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of the field of 3C 294.
Ref:	=2001MNRAS.322L..11F
by	FABIAN A.C. , CRAWFORD C.S., ETTORI S., SANDERS J.S.
	Mon. Not. R. Astron. Soc., 322, 11-15 (2001)
	Chandra detection of the intracluster medium around 3C 294 at z=1.786.
o	Text: <[FCE2001] JHHMMSS.sss+DDMMSS.ss> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCE2013]
[FCE2013]	(Fan+Chen+Er+, 2013)
Write:	<<[FCE2013] NN>> <<[FCE2013] PEG-NN>> (not recognised by Simbad, but found in literature)
N:	10
Object:	Grav. lensed image of a G (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=10 massive lensed passively evolving galaxies (PEGs). Use of HST CLASH and Spitzer IRAC data.
Ref:	=2013MNRAS.431L..15F
by	FAN L. , CHEN Y., ER X., LI J., LIN L., KONG X.
	Mon. Not. R. Astron. Soc., 431L, 15-19 (2013)
	Large size scatter of passively evolving lensed galaxies at z ~ 2 in CLASH.
o	Table 1: <[FCE2013] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCF2013]
[FCF2013]	(Fu+Cooray+Feruglio+, 2013) (Not yet in Simbad)
Write:	<<[FCF2013] X01W>>
N:	2
Object:	smm G (SIMBAD class: Galaxy)
Note:	SMA and JVLA observations of N=2 massive submillimetre bright merging galaxies.
in source:	1HERMES S250 J022016.0-060143
Ref:	=2013Natur.498..338F
by	FU H. , COORAY A., FERUGLIO C., IVISON R.J., RIECHERS D.A., GURWELL M., BUSSMANN R.S., HARRIS A., ALTIERI B., AUSSEL H., BAKER A.J., BOCK J., BOYLAN-KOLCHIN M., BRIDGE C., CALANOG J.A., CASEY C.M., CAVA A., CHAPMAN S.C., CLEMENTS D.L., CONLEY A., COX P., FARRAH D., FRAYER D., HOPWOOD R., JIA J., MAGDIS G., MARSDEN G., MARTINEZ-NAVAJAS P., NEGRELLO M., NERI R., OLIVER S.J., OMONT A., PAGE M.J., PEREZ-FOURNON I., SCHULZ B., SCOTT D., SMITH A., VACCARI M., VALTCHANOV I., VIEIRA J.D., VIERO M., WANG L., WARDLOW J.L., ZEMCOV M.
	Natur, 498, 338-341 (2013)
	The rapid assembly of an elliptical galaxy of 400 billion solar masses at a redshift of 2.3.
o	Table 1: SMM J105141 = [GIB2004] MM J105142+5719, SMM J123707/HDF 242 = NAME SMM J123707.21+621408.1 and SMM J123711/HDF 254 = NAME SMM J123711.32+621331.3.
o	Fig. 1: <[FCF2013] X01W> (Nos X01N, X01S).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FCG
FCG	(FIRST catalog radio Galaxy or component Group) (Not yet in Simbad)
Write:	<<FCG JHHMMSS.s+DDMMSS>>
N:	over 2000
Object:	Radio G (SIMBAD class: RadioG = Radio Galaxy)
Note:	Identification of various morphological types of galaxies in the FIRST Survey. Since the FIRST catalogs are catalogs of components, it would be useful to have coordinate and size estimates for various types of radio galaxies, e.g. Wide-Angle Tail, Narrow-Angle Tail, HYMORE, and Double-Doubles that consist of multiple components. While many of the groups have a component identifiable as a 'core' and are thus in the FIRST catalog, for a significant fraction there is no identifiable radio component at the expected core position. Other related publications: Proctor, D. D. 2002, J. Electron. Imaging, 12, 398 (2003JEI....12..398P) Low Resolution Pattern Recognition - Sorting Triples in the FIRST Database. Use of Morphological Annotations for Groups in the FIRST Database. Proctor, D. D. 2006, Astrophys. J., Suppl. Ser., 165, 95 (2006ApJS..165...95P) Comparing Pattern Recognition Feature Sets for Sorting Triples in the FIRST Database. See also FIRST.
Ref:	=2011ApJS..194...31P
by	PROCTOR D.D.
	Astrophys. J., Suppl. Ser., 194, 31 (2011)
	Morphological annotations for groups in the FIRST database.
o	Tables 1-15: <FCG JHHMMSS.s+DDMMSS> N=1932. Institute of Geophysics and Planetary Physics, Lawrence Livermore National Laboratory
=E=	Catalogue in electronic form as J/ApJS/194/31
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
History	of this Acronym: replaces F03G
Details on Acronym: [FCG2011]
[FCG2011]	(Fernandez-Lopez+Curiel+Girart+, 2011)
Write:	<<[FCG2011] MMN>> <<[FCG2011] MM2W>>
N:	2+2
Object:	Core (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	SMA observations of the GGD 27 system.
in source:	GGD 27
Ref:	=2011AJ....141...72F
by	FERNANDEZ-LOPEZ M. , CURIEL S., GIRART J.M., HO P.T.P., PATEL N., GOMEZ Y.
	Astron. J., 141, 72 (2011)
	Millimeter and submillimeter high angular resolution interferometric observations: dust in the heart of IRAS 18162-2048.
o	Fig. 1, Table 3: <[FCG2011] MMN> (Nos MM1-MM2), <[FCG2011] MM2W> (Nos MM2E, MM2W).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCJ2003]
[FCJ2003]	(Feldmeier+Ciardullo+Jacoby+, 2003)= ([FCJ2003a])
Write:	<<[FCJ2003] F-NN>>
N:	69+16+75+12+7+16+77+46
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	Kitt Peak observations. Intracluster PNs in 8 fields in the Virgo Cluster.
in source:	NAME Virgo Cluster
Ref:	=2003ApJS..145...65F
by	FELDMEIER J.J. , CIARDULLO R., JACOBY G.H., DURRELL P.R.
	Astrophys. J., Suppl. Ser., 145, 65-81 (2003)
	Intracluster planetary nebulae in the Virgo cluster. II. Imaging catalog.
o	Table 6: <[FCJ2003] 1-NN> (Nos 1-1 to 1-69), <[FCJ2003] 2-NN> (Nos 2-1 to 2-16), <[FCJ2003] 3-NN> (Nos 3-1 to 3-75), <[FCJ2003] 4-NN> (Nos 4-1 to 4-12), <[FCJ2003] 5-N> (Nos 5-1 to 5-7), <[FCJ2003] 6-NN> (Nos 6-1 to 6-16), <[FCJ2003] 7-NN> (Nos 7-1 to 7-77), <[FCJ2003] 8-NN> (Nos 8-1 to 8-46).
=E=	Catalogue in electronic form as J/ApJS/145/65
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCJ2003a]
[FCJ2003a]	(Feldmeier+Ciardullo+Jacoby+, 2003)
*****	Avoid the usage of [FCJ2003a], prefer [FCJ2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCJ2003b]
[FCJ2003b]	(Ferrarese+Cote+Jordan, 2003)
Write:	<<[FCJ2003b] NN>>
N:	9
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of M 49: search for novae.
in source:	M 49 = NGC 4472
Ref:	=2003ApJ...599.1302F
by	FERRARESE L. , COTE P., JORDAN A.
	Astrophys. J., 599, 1302-1319 (2003)
	Hubble Space Telescope observations of novae in M49.
o	Table 2: <[FCJ2003b] AN> (Nos N1-N9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCJ97]
[FCJ97]	(Feldmeier+Ciardullo+Jacoby, 1997)
Write:	<<[FCJ97] M 101 NN>> <<[FCJ97] M 51 NN>> <<[FCJ97] M 96 NN>>
N:	65+64+74
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	See also: Ford, [JCF89], [CJF89], [JCF90], [CJH91], [MCJ93], [JCH96], [CJF98]
in source:	M 101 = NGC 5457
in source:	M 51 = NGC 5194
in source:	M 96
Ref:	=1997ApJ...479..231F
by	FELDMEIER J.J. , CIARDULLO R., JACOBY G.H.
	Astrophys. J., 479, 231-243 (1997)
	Planetary nebulae as standard candles. XI. Application to spiral galaxies.
o	Table 2: <[FCJ97] M 101 NN> (Nos 1-65). Table 3: <[FCJ97] M 51 NN> (Nos 1-64). Table 4: <[FCJ97] M 96 NN> (Nos 1-74)
=E=	Catalogue in electronic form as J/ApJ/479/231
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCK2002]
[FCK2002]	(Faure+Courbin+Kneib+, 2002)
Write:	<<[FCK2002] A>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Lensing system of the QSO SBSG 1520+530: 'L' is the lensing galaxy, 'M' and 'N' are 2 galaxies in the field of SBSG 1520+530. See also [CVS97], [CSB98].
in source:	SBSG 1520+530
Ref:	=2002A&A...386...69F
by	FAURE C. , COURBIN F., KNEIB J.P., ALLOIN D., BOLZONELLA M., BURUD I.
	Astron. Astrophys., 386, 69-76 (2002)
	The lensing system towards the doubly imaged quasar SBS 1520+530.
o	Fig.1: quasars A and B, Stars SE, NW = [CVS97] objects.
o	Fig.1: <[FCK2002] A> (Nos L, M, N>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCK2012]
[FCK2012]	(Ferreras+Cropper+Kawata+, 2012)
Write:	<<[FCK2012] NNN>>
N:	787
Object:	(UV) + Star Forming Region (SIMBAD class: UV = UV-emission Source)
Note:	Swift UVOT observations of N=787 star-forming regions in NGC 4321. Use of SDSS, KPNO/Hα and Spitzer IRAC imaging.
in source:	NGC 4321
Ref:	=2012MNRAS.424.1636F
by	FERRERAS I. , CROPPER M., KAWATA D., PAGE M., HOVERSTEN E.A.
	Mon. Not. R. Astron. Soc., 424, 1636-1646 (2012)
	The Swift/UVOT catalogue of NGC4321 star-forming sources: a case against density wave theory.
o	Tables 2-3: <[FCK2012] NNN> (Nos 1-787).
=E=	Catalogue in electronic form as J/MNRAS/424/1636
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCM2009]
[FCM2009]	(Finkelstein+Cohen+Malhotra+, 2009)
Write:	<<[FCM2009] CDFSN>> <<[FCM2009] EGSNN>>
N:	3+27
Object:	LAE G (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Analysis of N=30 Lyman-alpha emitting galaxies, selected from GALEX. Use of AEGIS, CFHTLS and MUSYC data. See also [DSB2008].
in source:	NAME Extended Chandra Deep Field South
in source:	NAME Extended Groth Strip
Ref:	=2009ApJ...700..276F
by	FINKELSTEIN S.L. , COHEN S.H., MALHOTRA S., RHOADS J.E.
	Astrophys. J., 700, 276-283 (2009)
	Evolution of Lyα galaxies: stellar populations at z ~ 0.3.
o	Table 1: <[FCM2009] CDFSN> (Nos CDFS1-CDFS3), <[FCM2009] EGSNN> (Nos EGS1-EGS27).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCM84]
[FCM84]	(Felli+Churchwell+Massi, 1984)
Write:	<<[FCM84] M17 UC-1>> <<[FCM84] M17 W-Bar>> <<[FCM84] M17 Arc>> <<[FCM84] M17 NN>>
N:	1+2+1+13
Object:	Region (SIMBAD class: Region = Region defined in the Sky)
Stat:	is completely incorporated in Simbad
Note:	N=1 Ultra Compact HII region, format 'M17 UC-1'. N=2 Bar regions, formats 'M17 N-Bar' and 'M17 S-Bar'. N=1 Arc, and N=13 Clumps (Nos 1-13).
in source:	M 17 = NGC 6618
Ref:	=1984A&A...136...53F
by	FELLI M. , CHURCHWELL E., MASSI M.
	Astron. Astrophys., 136, 53-64 (1984)
	A high resolution study of M 17 at 1.3, 2, 6 and 21 cm.
o	<[FCM84] M17 UC-1> N=1, <[FCM84] M17 N-Bar> N=1, <[FCM84] M17 S-Bar> N=1, <[FCM84] M17 Arc> N=1. Table 3, Fig.5: <[FCM84] M17 NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FCOS
FCOS	(Fornax, Compact Object Survey)
Write:	<<FCOS F-NNNN>>
N:	120+185
Object:	* + GlC + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	In the FCOS, compact objects in different fields of view towards the Fornax Cluster of Galaxies have been investigated spectroscopically using the 2.5m du Pont telescope at LCO in WFCCD multi-slit mode. The magnitude range covered was 19 < V < 21 mag, corresponding to -12.3 < M-V < -10.3 mag. The aim was to spectroscopically determine cluster membership for the observed sources to investigate the bright end of the globular cluster luminosity function of the central Fornax giant elliptical galaxy NGC 1399. The question was whether there is an significant overlap between the LF of the newly discovered UCOs (e.g. Phillipps+ 2001ApJ...560..201P) and the brightest GCs. Our results show that the overlap is significant and consistent with the UCOs being bright globular clusters (GCs).
in source:	NAME Fornax Cluster
Ref:	=2002A&A...383..823M
by	MIESKE S. , HILKER M., INFANTE L.
	Astron. Astrophys., 383, 823-837 (2002)
	Ultra compact objects in the Fornax cluster of galaxies: Globular clusters or dwarf galaxies?
o	Tables 2, A1, A2: <FCOS F-NNNN> N=120+185.
Ref:	=2004A&A...418..445M
by	MIESKE S. , HILKER M., INFANTE L.
	Astron. Astrophys., 418, 445-458 (2004)
	Fornax compact object survey FCOS: On the nature of Ultra Compact Dwarf galaxies.
o	Table 1: <FCOS F-NNNN> N=280.
=E=	Catalogue in electronic form as J/A+A/383/823
=E=	Catalogue in electronic form as J/A+A/418/445
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: FCP18
FCP18	(Fenech+Clark+Prinja, 2018)
Write:	<<FCP18 NNNA>>
N:	101+12
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	ALMA 3mm continuum observations of N=101+12 sources in the Galactic cluster Westerlund 1. The suffix A in format indicates knots of emission in extended sources.
in source:	Cl Westerlund 1
Ref:	=2018A&A...617A.137F
by	FENECH D.M. , CLARK J.S., PRINJA R.K., DOUGHERTY S., NAJARRO F., NEGUERUELA I., RICHARDS A., RITCHIE B.W., ANDREWS H.
	Astron. Astrophys., 617A, 137-137 (2018)
	An ALMA 3 mm continuum census of Westerlund 1.
o	Tables 3+A.1: <FCP18 NNNA> N=101+12 among (Nos 1-101).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FCP2006]
[FCP2006]	(Folatelli+Contreras+Phillips+, 2006) (Not yet in Simbad)
Write:	<<[FCP2006] CNN>>
N:	14
Object:	* (SIMBAD class: Star)
Note:	Comparison stars in the field of SN 2005BF.
Ref:	=2006ApJ...641.1039F
by	FOLATELLI G. , CONTRERAS C., PHILLIPS M.M., WOOSLEY S.E., BLINNIKOV S., MORRELL N., SUNTZEFF N.B., LEE B.L., HAMUY M., GONZALEZ S., KRZEMINSKI W., ROTH M., LI W., FILIPPENKO A.V., FOLEY R.J., FREEDMAN W.L., MADORE B.F., PERSSON S.E., MURPHY D., BOISSIER S., GALAZ G., GONZALEZ L., McCARTHY P.J., McWILLIAM A., PYCH W.
	Astrophys. J., 641, 1039-1050 (2006)
	SN 2005bf: a possible transition event between type Ib/c supernovae and γ-ray bursts.
o	Parag. 5 : GRB 990425 is a misprint for 980425
o	FIg.1, Table 1: <[FCP2006] CNN> (Nos C1-C14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCP2009]
[FCP2009]	(Finoguenov+Connelly+Parker+, 2009)
Write:	<<[FCP2009] XHHhNN>>
N:	25
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	X-ray detected galaxy groups in the CNOC2 survey. See also CNOC2XGG.
Ref:	=2009ApJ...704..564F
by	FINOGUENOV A. , CONNELLY J.L., PARKER L.C., WILMAN D.J., MULCHAEY J.S., SAGLIA R.P., BALOGH M.L., BOWER R.G., McGEE S.L.
	Astrophys. J., 704, 564-575 (2009)
	The roadmap for unification in galaxy group selection. I. A search for extended X-ray emission in the CNOC2 survey.
o	Table 1: <[FCP2009] XHHhNN> (Nos X14h01-X14h09, X21h01-X21h16) = <CNOC2XGG JHHMMSS+DDMM.m> N=25.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCS2011]
[FCS2011]	(Furuya+Cesaroni+Shinnaga, 2011)
Write:	<<[FCS2011] SMAN>>
N:	3 (SIMBAD class: denseCore = Dense Core)
Note:	SMA 335GHz observations of the high-mass star forming region GAL 019.61-00.23.
in source:	GAL 019.61-00.23
Ref:	=2011A&A...525A..72F
by	FURUYA R.S. , CESARONI R., SHINNAGA H.
	Astron. Astrophys., 525A, 72-72 (2011)
	Infall, outflow, and rotation in the G19.61-0.23 hot molecular core.
o	Table 3 : <[FCS2011] SMAN> (Nos SMA1-SMA3) N=3
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FCSS
FCSS	(Fornax Cluster Spectroscopic Survey)
Write:	<<FCSS JHHMMSS.s+DDMMSS>>
N:	about 7000
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	The Fornax Spectroscopic Survey is using the Two degree Field spectrograph (2dF) of the Anglo-Australian Telescope to obtain the first complete spectroscopic sample of the central region of the Fornax cluster. The survey is unique in that all objects (both ``stars'' and ``galaxies'') brighter than Bj=19.7 are measured. We expect to observe two complete 2dF fields, about 6 square degrees or 6000 objects, most of which will be Galactic stars and background galaxies and QSOs, as well as around 100 cluster galaxies. A full description of the survey is given in Drinkwater et al. (2000A&A...355..900D). The type of object could be "everything", as galactic stars, all types of galaxies, QSOs, and even what may be inter-galactic globular clusters in the Fornax cluster. 2007A&A...476...59M: first ref. with FCSS objects.
Ref:	=2007A&A...476...59M
by	MORRIS R.A.H. , PHILLIPPS S., JONES J.B., DRINKWATER M.J., GREGG M.D., COUCH W.J., PARKER Q.A., SMITH R.M.
	Astron. Astrophys., 476, 59-62 (2007)
	2MASS galaxies in the Fornax cluster spectroscopic survey.
o	Catalog: <FCSS JHHMMSS.s+DDMMSS> N=228+114.
=E=	Catalogue in electronic form as J/A+A/476/59
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [FCT2000]
[FCT2000]	(Felli+Comoretto+Testi+, 2000) (Not yet in Simbad)
Write:	<<[FCT2000] ANNN>>
N:	459
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Search for YSO in 5 ISOGAL fields (Nos A-E), letter 'A' to 'E' in the format.
Ref:	=2000A&A...362..199F
by	FELLI M. , COMORETTO G., TESTI L., OMONT A., SCHULLER F.
	Astron. Astrophys., 362, 199-214 (2000)
	The search for YSOs from ISOGAL data. Application to the l=+45 field.
o	Table 4: <[FCT2000] ANNN> (Nos A001-A046), <[FCT2000] BNNN> (Nos B001-B120), <[FCT2000] CNNN> (Nos C001-C187), <[FCT2000] DNNN> (Nos D001-D045), <[FCT2000] ENNN> (Nos E001-E061).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCT2005]
[FCT2005]	(Furuya+Cesaroni+Takahashi+, 2005)
Write:	<<[FCT2005] A>> <<[FCT2005] HC>>
N:	9+1
Object:	HII + Hot Core (SIMBAD class: HIIReg = HII Region)
Note:	Owens Valley and Nobeyama Radio Observatory interferometric observations toward the HII region [WC89] 019.61-0.23: N=9 UC HII regions, and 1 hot core (HC). Additional SEST SIMBA observations. Use of VLA archival data.
in source:	[WC89] 019.61-0.23
Ref:	=2005ApJ...624..827F
by	FURUYA R.S. , CESARONI R., TAKAHASHI S., MOMOSE M., TESTI L., SHINNAGA H., CODELLA C.
	Astrophys. J., 624, 827-831 (2005)
	Relative evolutionary timescale of hot molecular cores with respect to ultracompact H II regions.
o	Fig.2, Table 1: <[FCT2005] A> (Nos A-D, F-G, I-K), <[FCT2005] AA> (No. HC).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCT2008]
[FCT2008]	(Furuya+Cesaroni+Takahashi+, 2008)
Write:	<<[FCT2008] GLL.ll+B.bbA>>
N:	3+3
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	OVRO, NMA, and IRAM PdBI mm observations of three star-forming regions.
in source:	GAL 023.01-00.41
in source:	GAL 016.59-00.05
in source:	GAL 028.87+00.07
Ref:	=2008ApJ...673..363F
by	FURUYA R.S. , CESARONI R., TAKAHASHI S., CODELLA C., MOMOSE M., BELTRAN M.T.
	Astrophys. J., 673, 363-381 (2008)
	Candidate rotating toroids around high-mass (Proto)Stars.
o	Table 3: <[FCT2008] GLL.ll+B.bbA> N=3+3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCT2012]
[FCT2012]	(Fiorentino+Contreras Ramos+Tolstoy+, 2012)
Write:	<<[FCT2012] VNNN>> <<[FCT2012] CN>>
N:	416+7
Object:	RR Lyr + Cepheid (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=416 RR Lyr stars and N=7 Cepheids in M32. Use of archival multi-epoch HST ACS and WFC images in the F606W and F814W filters.
in source:	M 32
Ref:	=2012A&A...539A.138F
by	FIORENTINO G. , CONTRERAS RAMOS R., TOLSTOY E., CLEMENTINI G., SAHA A.
	Astron. Astrophys., 539A, 138-138 (2012)
	The ancient stellar population of M 32: RR Lyrae variable stars confirmed.
o	Table 2: <[FCT2012] VNNN> (Nos V1-V416). Table 3: <[FCT2012] CN> (Nos C1-C7).
=E=	Catalogue in electronic form as J/A+A/539/A138
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FCW
FCW	(Feigelson+Carkner+Wilking)
*****	Avoid the usage of FCW, prefer [FCW98]
Origin	of the Acronym: L (2008ApJ...687..406C)
Details on Acronym: [FCW98]
[FCW98]	(Feigelson+Carkner+Wilking, 1998)= (FCW)
Write:	<<[FCW98] N>>
N:	8
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Around [TS84] IRS 5
Ref:	=1998ApJ...494L.215F
by	FEIGELSON E.D. , CARKNER L., WILKING B.A.
	Astrophys. J., 494, 215-218 (1998)
	Circularly polarized radio emission from an X-ray protostar.
o	In abstract : IRS 5 is [TS84] IRS 5
o	Table 1: <[FCW98] N> (Nos 1-8)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCY2004]
[FCY2004]	(Frayer+Chapman+Yan+, 2004)
Write:	<<[FCY2004] NNNA>>
N:	28
Object:	Radio G (SIMBAD class: Galaxy)
Note:	Sub-mm and IR observations of 28 radio-selected galaxies in the Spitzer First Look Survey verification field.
Ref:	=2004ApJS..154..137F
by	FRAYER D.T. , CHAPMAN S.C., YAN L., ARMUS L., HELOU G., FADDA D., MORGANTI R., GARRETT M.A., APPLETON P., CHOI P., FANG F., HEINRICHSEN I., IM M., LACY M., MARLEAU F., MASCI F.J., SHUPE D.L., SOIFER B.T., SQUIRES G.K., STORRIE-LOMBARDI L.J., SURACE J.A., TEPLITZ H.I., WILSON G.
	Astrophys. J., Suppl. Ser., 154, 137-141 (2004)
	Infrared properties of radio-selected submillimeter galaxies in the Spitzer first look survey verification field.
o	Table 1: <[FCY2004] NNNA> N=28 among (Nos 1-211).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FCZ2012]
[FCZ2012]	(Fontani+Caselli+Zhang+, 2012)
Write:	<<[FCZ2012] AN>>
N:	2 (SIMBAD class: denseCore = Dense Core)
Note:	VLA NH3 observations of the field of IRAS 05345+3157.
in source:	NAME NGC 1985 IR Cluster
Ref:	=2012A&A...541A..32F
by	FONTANI F. , CASELLI P., ZHANG Q., BRAND J., BUSQUET G., PALAU A.
	Astron. Astrophys., 541A, 32-32 (2012)
	Temperature and kinematics of protoclusters with intermediate and high-mass stars: the case of IRAS 05345+3157.
o	Table 1: <[FCZ2012] AN> (Nos A1-A2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FD
FD	(Foley+Davis) (Not yet in Simbad)
*****	Avoid the usage of FD, prefer [FD85]
Origin	of the Acronym: L (1988A&A...198...87F)
Details on Acronym: FD
FD	(Fehrenbach+Duflot+)= (FDA)
Write:	<<FD NN>>
N:	80
Object:	WR (SIMBAD class: WolfRayet* = Wolf-Rayet)
Note:	N=80 (among which 6 are new), see ref. 1981A&AS...43..203B. Identif. charts only for Nos 50, 51, 53, 56, 77.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1976A&AS...24..379F
by	FEHRENBACH C. , DUFLOT M., ACKER A.
	Astron. Astrophys., Suppl. Ser., 24, 379-388 (1976)
	Les etoiles Wolf-Rayet dans le Grand Nuage de Magellan.
o	Table 2: <FD NN> (Nos 1-80)
Details on Acronym: FD
FD	(Faber+Dressler)
*****	Avoid the usage of FD, prefer [FD77]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: FD
FD	(Fehrenbach+Duflot)
*****	Avoid the usage of FD, prefer GV
Origin	of the Acronym: L (1997A&AS..121..247G)
Details on Acronym: FD
FD	(Fehrenbach+Duflot)
*****	Avoid the usage of FD, prefer PV
Origin	of the Acronym: L (1997A&AS..121..247G)
Details on Acronym: [FD70]
[FD70]	(Fehrenbach+Duflot, 1970)= (FDS) = (S)
Write:	<<[FD70] SNNN>>
N:	110
Object:	* (SIMBAD class: Star)
Note:	Supplementary list of galactic stars and stars in the LMC. See also GV and PV. Identif. charts
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1970A&ASS...1....1F
by	FEHRENBACH C. , DUFLOT M.
	Astron. Astrophys., Special Suppl. Ser., 1, 1-67 (1970)
	Grand Nuage de Magellan. Liste des etoiles membres du Grand Nuage de Magellan et liste d'etoiles galactiques.
o	<GV NNN> (Nos 1-495). <PV NNNN> (Nos 1-1830). <[FD70] SNNN> (Nos S1-S110).
Details on Acronym: [FD77]
[FD77]	(Faber+Dressler, 1977)= (FD)
Write:	<<[FD77] ACO NNNN NN>> <<[FD77] ACO 2256 A>>
N:	161
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Table I: G in 11 aco ClG. ACO 98: (Nos 1-13), format 'ACO 98 NN'. ACO 154: (Nos 1-12), format 'ACO 154 NN'. ACO 168: (Nos 1-13), format 'ACO 168 NN'. ACO 262: (Nos 1-13), format 'ACO 262 NN'. ACO 665: (Nos 1-4), format 'ACO 665 N'. ACO 754: (Nos 1-11), format 'ACO 754 NN'. ACO 1060: (Nos 1-11), format 'ACO 1060 NN'. ACO 1940: (Nos 1-20), format 'ACO 1940 NN'. ACO 2029: (Nos 1-18), format 'ACO 2029 NN'. ACO 2256: N=14 among (Nos A-X), format 'ACO 2256 A'. ACO 2319: (Nos 1-35), format 'ACO 2319 NN'.
in source:	ACO 98
in source:	ACO 154
in source:	ACO 168
in source:	ACO 262
in source:	ACO 665
in source:	ACO 754
in source:	ACO 1060
in source:	ACO 1940
in source:	ACO 2029
in source:	ACO 2256
in source:	ACO 2319
Ref:	=1977AJ.....82..187F
by	FABER S.M. , DRESSLER A.
	Astron. J., 82, 187-192 (1977)
	Radial velocities for galaxies in 11 clusters.
o	Table I: <[FD77] ACO NNNN NN> N=147, <[FD77] ACO 2256 A> N=14 among (Nos A-X)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FD82]
[FD82]	(Fehrenbach+Duflot, 1982)= (FDG) = (G)
Write:	<<[FD82] NNN>>
N:	711
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Liste G, 1st col., cross id. with GV designation in 2nd col.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1982A&AS...48..409F
by	FEHRENBACH C. , DUFLOT M.
	Astron. Astrophys., Suppl. Ser., 48, 409-442 (1982)
	Vitesses radiales au prisme objectif dans la direction du Grand Nuage de Magellan.
o	revision of <GV NNN> and <PV NNNN>. New numbering for GV list: <[FD82] NNN> (Nos 1-711).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FD85]
[FD85]	(Foley+Davis, 1985)= (FD) (Not yet in Simbad)
Write:	<<[FD85] N>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	MERLIN observations of the radio jet of the QSO 3C 273.
in source:	3C 273
Ref:	=1985MNRAS.216..679F
by	FOLEY A.R. , DAVIS R.J.
	Mon. Not. R. Astron. Soc., 216, 679-690 (1985)
	MERLIN radio observations of the quasar 3C 273.
o	Fig.1, Table 1: <[FD85] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FDA
FDA	(Fehrenbach+Duflot+Acker)
*****	Avoid the usage of FDA, prefer FD
Origin	of the Acronym: L (2002ApJS..141...81M)
Details on Acronym: [FDB2011]
[FDB2011]	(Favre+Despois+Brouillet+, 2011)
Write:	<<[FDB2011] MFNN>> <<[FDB2011] CaN>>
N:	28+6
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	IRAM Plateau de Bure Interferometer observations of N=28 methyl formate ({bf MF) emission peaks and N=6 dust clumps.

in source:	NAME Orion KL
Ref:	=2011A&A...532A..32F
by	FAVRE C. , DESPOIS D., BROUILLET N., BAUDRY A., COMBES F., GUELIN M., WOOTTEN A., WLODARCZAK G.
	Astron. Astrophys., 532A, 32-32 (2011)
	HCOOCH_{3} as a probe of temperature and structure in Orion-KL.
o	Fig. 4, Table 2: <[FDB2011] MFNN> (Nos MF1-MF28). Fig. 16, Tables 7-8: <[FDB2011] CaN> (Nos Ca-Cd, Cb1-Cb2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FDC2002]
[FDC2002]	(Fiaschi+Di Mille+Cariolato+, 2002)
Write:	<<[FDC2002] JHHMMSS.ss+DDMMSS.s>>
N:	3
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Stat:	is completely incorporated in Simbad
Note:	Astronomical Observatory G. Colombo and LOTOSS observations. Discovery of three new novae in M 31.
in source:	M 31 = NGC 224
Ref:	=2002IAUC.7794....1F
by	FIASCHI M. , DI MILLE F., CARIOLATO R., SWIFT B., LI W.D., LOTOSS
	IAU Circ., 7794, 1-None (2002)
	Novae in M 31.
o	<[FDC2002] JHHMMSS.ss+DDMMSS.s> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FDD81]
[FDD81]	(Fishman+Duthie+Dufour, 1981)
Write:	<<[FDD81] GRB 781119 NN>> <<[FDD81] GRB 790305 N>>
N:	22+8
Object:	* (SIMBAD class: Star)
Note:	Fig.1, Table I: N=22 stars in the region of GRB 781119. Fig.2, Table II: N=8 stars in the region of GRB 790305B.
Ref:	=1981Ap&SS..75..135F
by	FISHMAN G.J. , DUTHIE J.G., DUFOUR R.J.
	Astrophys. Space Sci., 75, 135-None (1981)
	Optical studies on the regions of the γ-ray bursts of Nov. 19, 1978 and March 5, 1979.
o	Fig.1, Table I: <[FDD81] GRB 781119 NN> (Nos 1-22). Fig.2, Table II: <[FDD81] GRB 790305 N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FDE2007]
[FDE2007]	(Firth+Drinkwater+Evstigneeva+, 2007)
Write:	<<[FDE2007] JHHMMSS.ss+DDMMSS.s>>
N:	32+27
Object:	Compact Stellar System (SIMBAD class: Cluster* = Cluster of Stars)
Note:	VLT-FLAMES search for CSS (Compact Stellar System) in the Fornax Cluster.
in source:	NAME Fornax Cluster
Ref:	=2007MNRAS.382.1342F
by	FIRTH P. , DRINKWATER M.J., EVSTIGNEEVA E.A., GREGG M.D., KARICK A.M., JONES J.B., PHILLIPPS S.
	Mon. Not. R. Astron. Soc., 382, 1342-1352 (2007)
	Compact stellar systems around NGC1399.
o	In Chap. 4. : UCD 3 = FCOS 1-2053, In chap 2.4 : UCD 22 = FCOS 4-2028.
o	Table 2: <[FDE2007] JHHMMSS.ss+DDMMSS.s> N=32+27.
=E=	Catalogue in electronic form as J/MNRAS/382/1342
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FDF
FDF	(FORS Deep Field)
Write:	<<FDF NNNN>>
N:	9011
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT observations. Photometric catalog of objects in the FORS Deep Field.
in source:	NAME FDF
Ref:	=2003A&A...398...49H
by	HEIDT J. , APPENZELLER I., GABASCH A., JAEGER K., SEITZ S., BENDER R., BOEHM A., SNIGULA J., FRICKE K.J., HOPP U., KUEMMEL M., MOELLENHOFF C., SZEIFERT T., ZIEGLER B., DRORY N., MEHLERT D., MOORWOOD A., NICKLAS H., NOLL S., SAGLIA R.P., SEIFERT W., STAHL O., SUTORIUS E., WAGNER S.J.
	Astron. Astrophys., 398, 49-61 (2003)
	The FORS Deep Field: Field selection, photometric observations and photometric catalog.
o	Table 4: <FDF NNNN> (Nos 1-8753).
Ref:	=2004A&A...418..885N
by	NOLL S. , MEHLERT D., APPENZELLER I., BENDER R., BOEHM A., GABASCH A., HEIDT J., HOPP U., JAEGER K., SEITZ S., STAHL O., TAPKEN C., ZIEGLER B.L.
	Astron. Astrophys., 418, 885-906 (2004)
	The FORS Deep Field spectroscopic survey.
o	Table 1: <FDF NNNN> N=341, N=6 added among (Nos 9002-9011).
=E=	Catalogue in electronic form as J/A+A/398/49
=E=	Catalogue in electronic form as J/A+A/418/885
Origin	of the Acronym: L (2002A&A...393..809M)
Details on Acronym: [FDF99]
[FDF99]	(Fontana+D'Odorico+Fosbury+, 1999)= (VLT)
Write:	<<[FDF99] VLT NNN>>
N:	7
Object:	Poss. G (SIMBAD class: Galaxy)
Note:	From ESO public archive. N=7 galaxy candidates from the VLT photometric catalogue of the HDFS obtained with the first VLT 8.2 telescope (UTI).
in source:	NAME HDFS
Ref:	=1999A&A...343L..19F
by	FONTANA A. , D'ODORICO S., FOSBURY R., GIALLONGO E., HOOK R., POLI F., RENZINI A., ROSATI P., VIEZZER R.
	Astron. Astrophys., 343, 19-24 (1999)
	The VLT observations of the HDF-S NICMOS field: photometric catalog and high redshift galaxy candidates.
o	Table 2, text: <[FDF99] VLT NNN> N=7 among (Nos 24-154).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FDG
FDG	(Fehrenbach+Duflot, G list)
*****	Avoid the usage of FDG, prefer [FD82]
Origin	of the Acronym: L (2002ApJS..141...81M)
Details on Acronym: [FDG2020]
[FDG2020]	(Forbes+Dullo+Gannon+, 2019)
Write:	<<[FDG2020] IC 1459 group UDGN>> <<[FDG2020] IC 1459 group LSBN>>
N:	12
Object:	Ultra-diffuse G + LSB Dwarf G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Identification of N=9 ultradiffuse galaxies (UDGs) and N=3 low surface brightness (LSB) galaxies in the IC 1459 group. Use of VST survey of Early-type GAlaxieS (VEGAS) imaging.
in source:	NAME IC 1459 Group
Ref:	=2020MNRAS.494.5293F
by	FORBES D.A. , DULLO B.T., GANNON J., COUCH W.J., IODICE E., SPAVONE M., CANTIELLO M., SCHIPANI P.
	Mon. Not. R. Astron. Soc., 494, 5293-5297 (2020)
	Ultradiffuse galaxies in the IC 1459 group from the VEGAS survey.
o	Tables 1-2: <[FDG2020] IC 1459 group UDGN> (Nos UDG1-UDG9), <[FDG2020] IC 1459 group LSBN> (Nos LSB1-LSB3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FDH2002]
[FDH2002]	(Foschini+Di Cocco+Ho+, 2002)
Write:	<<[FDH2002] NGC NNNN ULXN>>
N:	18
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton study of UltraLuminous X-ray (ULX) sources in a sample of 9 Seyfert galaxies.
in source:	NGC 1058
in source:	NGC 3185
in source:	NGC 3486
in source:	NGC 3941
in source:	NGC 4168
in source:	NGC 4501
in source:	NGC 4565
in source:	NGC 4639
in source:	NGC 4698
Ref:	=2002A&A...392..817F
by	FOSCHINI L. , DI COCCO G., HO L.C., BASSANI L., CAPPI M., DADINA M., GIANOTTI F., MALAGUTI G., PANESSA F., PICONCELLI E., STEPHEN J.B., TRIFOGLIO M.
	Astron. Astrophys., 392, 817-825 (2002)
	XMM-Newton observations of ultraluminous X-ray sources in nearby galaxies.
o	Table 2: <[FDH2002] NGC NNNN ULXN> N=18.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FDH2007]
[FDH2007]	(Fender+Dahlem+Homan+, 2007)
Write:	<<[FDH2007] A>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA 4.8GHz and 8.6GHz observations of XTE J1701-462. N=4 sources south of XTE are found.
Ref:	=2007MNRAS.380L..25F
by	FENDER R.P. , DAHLEM M., HOMAN J., CORBEL S., SAULT R., BELLONI T.M.
	Mon. Not. R. Astron. Soc., 380L, 25-29 (2007)
	The variable radio counterpart and possible large-scale jet of the new Z source XTE J1701-462.
o	Table 2, Fig.5: <[FDH2007] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FDK2002]
[FDK2002]	(Fox+Djorgovski+Kulkarni, 2002)
Write:	<<[FDK2002] GRB 020127 Host G>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck-II spectrographic observations of GRB 020127: detection of the host galaxy.
Ref:	=2002GCN..1306....1F
by	FOX D.W. , DJORGOVSKI S.G., KULKARNI S.R.
	GRB Coordinates Network, Circular Service, 1306, 1-None (2002)
	GRB020127: proposed host galaxy detection and identification of afterglow.
o	<[FDK2002] GRB 020127 Host G> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FDK2008]
[FDK2008]	(Firth+Drinkwater+Karick, 2008)
Write:	<<[FDK2008] JHHMMSS.ss+DDMMSS.s>>
N:	19+17
Object:	Compact Stellar System (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	AAOmega (AAT) spectrograph observations of Virgo and Fornax clusters. Search for compact stellar systems (CSSs). See also: [DJG2000], [FDE2007], [GDE2009].
in source:	NAME Virgo Cluster
in source:	NAME Fornax Cluster
Ref:	=2008MNRAS.389.1539F
by	FIRTH P. , DRINKWATER M.J., KARICK A.M.
	Mon. Not. R. Astron. Soc., 389, 1539-1555 (2008)
	Compact stellar systems and cluster environments.
o	Tables 4, 5: <[FDK2008] JHHMMSS.ss+DDMMSS.s> N=19+17.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FDL2020]
[FDL2020]	(Fensch+Duc+Lim+, 2020)
Write:	<<[FDL2020] NGC 474 GCN>> <<[FDL2020] NGC 474 PNN>>
N:	6+8
Object:	Poss. GlCl + Poss. PN (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	VLT MUSE observations of N=6 globular cluster candidates and N=8 planetary nebula candidates in the outer shell of NGC 474.
in source:	NGC 474
Ref:	=2020A&A...644A.164F
by	FENSCH J. , DUC P.-A., LIM S., EMSELLEM E., BILEK M., DURRELL P., LIU C., PENG E., SMITH R.
	Astron. Astrophys., 644A, 164-164 (2020)
	Shedding light on the formation mechanism of shell galaxy NGC 474 with MUSE.
o	Fig. 1, Table 1: <[FDL2020] NGC 474 GCN> (Nos GC1-GC6), <[FDL2020] NGC 474 PNN> (Nos PN1-PN8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FDM2003]
[FDM2003]	(Flaccomio+Damiani+Micela+, 2003)
Write:	<<[FDM2003] X NNN>> <<[FDM2003] Opt NNN>>
N:	742+696
Object:	X + (Opt) (SIMBAD class: X = X-ray Source)
Note:	Chandra HRC-I observations of the Orion Nebula Cluster (ONC).
in source:	NAME ONC
Ref:	=2003ApJ...582..382F
by	FLACCOMIO E. , DAMIANI F., MICELA G., SCIORTINO S., HARNDEN F.R.Jr, MURRAY S.S., WOLK S.J.
	Astrophys. J., 582, 382-397 (2003)
	Chandra X-ray observation of the Orion Nebula Cluster. I. Detection, identification, and determination of X-ray luminosities.
o	p.391: source "n" = LBLS n (= [FDM2003] X 272).
o	Table 1: <[FDM2003] X NNN> (Nos 1-742). Table 4: <[FDM2003] Opt NNN> (Nos 1-696).
=E=	Catalogue in electronic form as J/ApJ/582/382
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FDP2000]
[FDP2000]	(Fontana+D'Odorico+Poli+, 2000)
Write:	<<[FDP2000] nNNNN>> <<[FDP2000] qNNNN>>
N:	347+120
Object:	G (SIMBAD class: Galaxy)
Note:	Photometric catalog of high redshift galaxies in NTTDF (NTT Deep Field): letter 'n' refers to NTTDF object, in BRI 1202-07 field: letter 'q' refers to this field.
in source:	NAME NTTDF
Ref:	=2000AJ....120.2206F
by	FONTANA A. , D'ODORICO S., POLI F., GIALLONGO E., ARNOUTS S., CRISTIANI S., MOORWOOD A., SARACCO P.
	Astron. J., 120, 2206-2219 (2000)
	Photometric redshifts and selection of high-redshift galaxies in the NTT and Hubble Deep Fields.
o	Fig.9: HDF-N-3259-652 not identified.
o	Table 2: <[FDP2000] nNNNN> N=347 among (Nos n0001-n0547), <[FDP2000] qNNNN> N=120 among (Nos q0002-q0449).
=E=	Catalogue in electronic form as J/AJ/120/2206
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FDQ
FDQ	(FIRST Deeprange QSO)
Write:	<<FDQ JHHMMSS.s+DDMMSS>>
N:	35+14
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	Sample of quasar candidates by comparing the FIRST radio survey with the 16deg2 Deeprange I-band survey (KPNO observations).
Ref:	=2003AJ....126..706W
by	WHITE R.L. , HELFAND D.J., BECKER R.H., GREGG M.D., POSTMAN M., LAUER T.R., OEGERLE W.
	Astron. J., 126, 706-722 (2003)
	An I-band-selected sample of radio-emitting quasars: evidence for a large population of red quasars.
o	Tabls 1, 2: <FDQ JHHMMSS.s+DDMMSS> N=35+14.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FDS
FDS	(Fehrenbach+Duflot, Suppl.)
*****	Avoid the usage of FDS, prefer [FD70]
Origin	of the Acronym: L (2002ApJS..141...81M)
Details on Acronym: FDS
FDS	(Fornax Deep Survey)
Write:	<<FDS JHHMMSS.ss+DDMMSS.ss>> <<FDS FF NNNNa>> <<FDS FF_NNNNa>> (not recognised by Simbad, but found in literature)
N:	1682503+3112605+582
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	ESO VLT Survey Telescope (VST) observations of 26 fields (numbered between 1 and 31) in the Fornax galaxy cluster, as part of the Fornax Deep Survey. 2020A&A...639A.136C: Format JHHMMSS.ss+DDMMSS.ss, N=1682503+3112605 sources . See also: http://fdscat.oa-abruzzo.inaf.it/ 2021A&A...647A.100S: Format FF NNNNa, N=582 galaxies. See also: https://www.oulu.fi/astronomy/FDS_DECOMP/main/index.html
in source:	NAME Fornax Cluster
Ref:	=2020A&A...639A.136C
by	CANTIELLO M. , VENHOLA A., GRADO A., PAOLILLO M., D'ABRUSCO R., RAIMONDO G., QUINTINI M., HILKER M., MIESKE S., TORTORA C., SPAVONE M., CAPACCIOLI M., IODICE E., PELETIER R., FALCON BARROSO J., LIMATOLA L., NAPOLITANO N., SCHIPANI P., VAN DE VEN G., GENTILE F., COVONE G.
	Astron. Astrophys., 639A, 136-136 (2020)
	The Fornax Deep Survey with VST. IX. Catalog of sources in the FDS area with an example study for globular clusters and background galaxies.
o	Tables 3-4: <FDS JHHMMSS.ss+DDMMSS.ss> N=1682503+3112605.
Ref:	=2021A&A...647A.100S
by	SU A.H. , SALO H., JANZ J., LAURIKAINEN E., VENHOLA A., PELETIER R.F., IODICE E., HILKER M., CANTIELLO M., NAPOLITANO N., SPAVONE M., RAJ M.A., VAN DE VEN G., MIESKE S., PAOLILLO M., CAPACCIOLI M., VALENTIJN E.A., WATKINS A.E.
	Astron. Astrophys., 647A, 100-100 (2021)
	The Fornax Deep Survey (FDS) with the VST. XI. The search for signs of preprocessing between the Fornax main cluster and Fornax A group.
o	<FDS FF NNNNa> N=582.
=E=	Catalogue in electronic form as <J/A+A/639/A136/>
=E=	Catalogue in electronic form as <J/A+A/647/A100/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FDS
FDS	(Fornax Deep Survey)
*****	Avoid the usage of FDS, prefer [VPL2017]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FDS
FDS	(Fornax Deep Survey)
*****	Avoid the usage of FDS, prefer [VPL2018]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FDS2009]
[FDS2009]	(Friesen+Di Francesco+Shirley+, 2009)
Write:	<<[FDS2009] AN-ANN>> <<[FDS2009] B1-C2S>> <<[FDS2009] C-C2S>> <<[FDS2009] C-HC5N>>
N:	21+3
Object:	NH3 Clump + Peak (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	ATCA, VLA and GBT observations of dense cores in Ophiuchus.
in source:	NAME rho Oph Cloud
in source:	NAME RHO OPH CLOUD:[LWS80] RHO OPH B1 = [LWS80] RHO OPH B1
in source:	NAME RHO OPH CLOUD:[LWS80] RHO OPH B2 = [LWS80] RHO OPH B2
in source:	NAME RHO OPH CLOUD:[LWS80] RHO OPH C = [LWS80] RHO OPH C
in source:	NAME RHO OPH CLOUD:[LWS80] RHO OPH F = [LWS80] RHO OPH F
Ref:	=2009ApJ...697.1457F
by	FRIESEN R.K. , DI FRANCESCO J., SHIRLEY Y.L., MYERS P.C.
	Astrophys. J., 697, 1457-1480 (2009)
	The initial conditions of clustered star formation. I. NH_{3}Observations of dense cores in Ophiuchus.
o	Tables 4, 8: <[FDS2009] AN-ANN> (Nos B1-A1 to B1-A4, B2-A1 to B2-A10, C-A1 to C-A3, F-A1 to F-A3). Table 5: <[FDS2009] B1-C2S> N=1, <[FDS2009] C-C2S> N=1, <[FDS2009] C-HC5N> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FDS2010]
[FDS2010]	(Friesen+Di Francesco+Shimajiri+, 2010)
Write:	<<[FDS2010] BNN-NN>>
N:	17
Object:	N2H+ clump (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	Nobeyama 45m radio telescope and ATCA observations of the Ophiuchus B core.
in source:	NAME rho Oph B Cloud
Ref:	=2010ApJ...708.1002F
by	FRIESEN R.K. , DI FRANCESCO J., SHIMAJIRI Y., TAKAKUWA S.
	Astrophys. J., 708, 1002-1024 (2010)
	The initial conditions of clustered star formation. II. N_{2}H^+ observations of the Ophiuchus B core.
o	Table 2: <[FDS2010] BNN-NN> (Nos B1-N1 to B1-N4, B12-N1 to B12-N3, B2-N1 to B2-N9, B3-N1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FDS2021]
[FDS2021]	(Froebrich+Derezea+Scholz+, 2021)
Write:	<<[FDS2021] NNNNN>>
N:	59
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	N=59 periodic variables in IC 5070, as part of the Hunting Outbursting Young Stars (HOYS) citizen science project. Use of Gaia EDR3 data.
in source:	NAME Pelican Nebula = IC 5070
Ref:	=2021MNRAS.506.5989F
by	FROEBRICH D. , DEREZEA E., SCHOLZ A., EISLOFFEL J., VANAVERBEKE S., KUME A., HERBERT C., CAMPBELL-WHITE J., MILLER N., STECKLUM B., MAKIN S.V., URTLY T., SOLDAN ALFARO F.C., SCHWENDEMAN E., STONE G., PHILLIPS M., FLEMING G., GONZALEZ FARFAN R., VANMUNSTER T., HEALD M.A., FERNANDEZ MANANES E., NELSON T., EGGENSTEIN H.-B., DUBOIS F., LOGIE L., RAU S., WIERSEMA K., QUINN N., RODRIGUEZ D., CASTILLO GARCIA R., KILLESTEIN T., VALE T., LICCHELLI D., DELDEM M., PIEHLER G., MOZDZIERSKI D., KOTYSZ K., KOWALSKA K., MIKOLAJCZYK P., FUTCHER S.R.L., LONG T.P., MORALES AIMAR M., MERRIKIN B., JOHNSTONE S., DUBOVSKY P.A., KUDZEJ I., PICKARD R., BILLINGTON S.J., DOVER L., ZEGMOTT T., EVITTS J.J., TRASPAS MUNIA A., PRICE M.C.
	Mon. Not. R. Astron. Soc., 506, 5989-6000 (2021)
	A survey for variable young stars with small telescopes - IV. Rotation periods of YSOs in IC 5070.
o	Tables 4-5: <[FDS2021] NNNNN> N=59 among (Nos 2287-11246).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FDT2003]
[FDT2003]	(Fiaschi+Di Mille+Tiveron, 2003)
Write:	<<[FDT2003] JHHMMSS.ss+DDMMSS.s>>
N:	2+1
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Stat:	is completely incorporated in Simbad
Note:	Astronomical Observatory G. Colombo observations. Discovery of two then one new novae in M 31.
in source:	M 31 = NGC 224
Ref:	=2003IAUC.8155....1F
by	FIASCHI M. , DI MILLE F., TIVERON D.
	IAU Circ., 8155, 1-None (2003)
	Novae in M31.
o	<[FDT2003] JHHMMSS.ss+DDMMSS.s> N=2.
Ref:	=2003IAUC.8238....2F
by	FIASCHI M. , DI MILLE F., TIVERON D.
	IAU Circ., 8238, 2-None (2003)
	Novae in M31.
o	<[FDT2003] JHHMMSS.ss+DDMMSS.s> N=1 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FEB2018]
[FEB2018]	(Franco+Elbaz+Bethermin+, 2018)
Write:	<<[FEB2018] AGSNN>>
N:	39
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ALMA 1.1mm observations of N=23 galaxies in the GOODS South field. Use of CANDELS (HST WFC3), Spitzer, Herschel, VLA, Chandra, and ALMA 1.3mm data. Nos AGS1-AGS23: Main Catalog (2018A&A...620A.152F) Nos AGS24-AGS39: Supplementary Catalog (2020A&A...643A.53F) See also [GEX2022].
in source:	NAME GOODS South Field
Ref:	=2018A&A...620A.152F
by	FRANCO M. , ELBAZ D., BETHERMIN M., MAGNELLI B., SCHREIBER C., CIESLA L., DICKINSON M., NAGAR N., SILVERMAN J., DADDI E., ALEXANDER D.M., WANG T., PANNELLA M., LE FLOC'H E., POPE A., GIAVALISCO M., MAURY A.J., BOURNAUD F., CHARY R., DEMARCO R., FERGUSON H., FINKELSTEIN S.L., INAMI H., IONO D., JUNEAU S., LAGACHE G., LEITON R., LIN L., MAGDIS G., MESSIAS H., MOTOHARA K., MULLANEY J., OKUMURA K., PAPOVICH C., PFORR J., RUJOPAKARN W., SARGENT M., SHU X., ZHOU L.
	Astron. Astrophys., 620A, 152-152 (2018)
	GOODS-ALMA: 1.1 mm galaxy survey. I. Source catalog and optically dark galaxies.
o	Fig. 1, Tables 2-3: <[FEB2018] AGSNN> (Nos 1-23).
Ref:	=2020A&A...643A..53F
by	FRANCO M. , ELBAZ D., ZHOU L., MAGNELLI B., SCHREIBER C., CIESLA L., DICKINSON M., NAGAR N., MAGDIS G., ALEXANDER D.M., BETHERMIN M., DEMARCO R., DADDI E., WANG T., MULLANEY J., INAMI H., SHU X., BOURNAUD F., CHARY R., COOGAN R.T., FERGUSON H., FINKELSTEIN S.L., GIAVALISCO M., GOMEZ-GUIJARRO C., IONO D., JUNEAU S., LAGACHE G., LIN L., MOTOHARA K., OKUMURA K., PANNELLA M., PAPOVICH C., POPE A., RUJOPAKARN W., SILVERMAN J., XIAO M.
	Astron. Astrophys., 643A, 53-53 (2020)
	GOODS-ALMA: Using IRAC and VLA to probe fainter millimeter galaxies.
o	Tables 1-2: <[FEB2018] AGSNN> (Nos 24-39).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FED2000]
[FED2000]	(Fadda+Elbaz+Duc+, 2000)
Write:	<<[FED2000] NN>>
N:	45
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	ISOCAM and ISOPHOT observations from ISO. N=45 objects in the field of ACO 1689: N=32 G in ACO, 5 background or foreground G, 6 stars, 1 QSO, 1 ?. Finding chart Fig.1.
in source:	ACO 1689
Ref:	=2000A&A...361..827F
by	FADDA D. , ELBAZ D., DUC P.-A., FLORES H., FRANCESCHINI A., CESARSKY C.J., MOORWOOD A.F.M.
	Astron. Astrophys., 361, 827-840 (2000)
	An excess of mid-IR luminous galaxies in Abell 1689?
o	in ref list Dwek 1997ApJ.475.565 instead of 1990
o	Table 2: <[FED2000] NN> (Nos 1-45).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Feig
Feig	(Feige)
====>	Equivalent to: Feige
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Feige
Feige	(Feige)= (F) = Feig
Write:	<<Feige NNN>>
N:	114
Object:	Blue * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	An Atlas of identification for 113 of these stars is given in ApJ 129, p. 600
Ref:	=1958ApJ...128..267F
by	FEIGE J.
	Astrophys. J., 128, 267-272 (1958)
	A search for underluminous hot stars.
o	<Feige NNN> (Nos 1-114).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Feigelson
Feigelson	(Feigelson+)
*****	Avoid the usage of Feigelson, prefer [FBG2002]
Origin	of the Acronym: L (2004AJ....128..787R)
Details on Acronym: Feinstein
Feinstein	(Feinstein)
Write:	<<Cl Feinstein N>> <<Cl Feinstein 1>>
N:	1
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Stat:	is completely incorporated in Simbad
Ref:	=1964Obs....84..111F
by	FEINSTEIN A.
	The Observatory, 84, 111-115 (1964)
	A group of stars around the He star HD 96446.
o	Table 1, col(1): numbering not in SIMBAD.
o	<Cl Feinstein 1>
Details on Acronym: [FEJ2006]
[FEJ2006]	(Firth+Evstigneeva+Jones+, 2006)
Write:	<<[FEJ2006] JHHMMSS.s+DDMMSS>>
N:	4
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Anglo-Australian Telescope 2dF observations of 6 nearby galaxy groups. In the group LGG 345, 4 new galaxies are found.
in source:	NAME LGG 345 = NAME NGC 5084 GROUP
Ref:	=2006MNRAS.372.1856F
by	FIRTH P. , EVSTIGNEEVA E.A., JONES J.B., DRINKWATER M.J., PHILLIPPS S., GREGG M.D.
	Mon. Not. R. Astron. Soc., 372, 1856-1868 (2006)
	Kinematics, substructure and luminosity-weighted dynamics of six nearby galaxy groups.
o	Table 12: <[FEJ2006] JHHMMSS.s+DDMMSS> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FEM2009]
[FEM2009]	(Feain+Ekers+Murphy+, 2009)
Write:	<<[FEM2009] JHHMMSS+DDMMSS>> <<[FEM2009] HHMMSS+DDMMSS>> (not recognised by Simbad, but found in literature)
N:	1005+281
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ATCA 1.4GHz continuum observations of Centaurus A.
in source:	Cen A = NGC 5128
Ref:	=2009ApJ...707..114F
by	FEAIN I.J. , EKERS R.D., MURPHY T., GAENSLER B.M., MacQUART J.-P., NORRIS R.P., CORNWELL T.J., JOHNSTON-HOLLITT M., OTT J., MIDDELBERG E.
	Astrophys. J., 707, 114-125 (2009)
	Faraday rotation structure on kiloparsec scales in the radio lobes of Centaurus A.
o	Tables 2-3: <[FEM2009] JHHMMSS+DDMMSS> N=1005+281.
=E=	Catalogue in electronic form as J/ApJ/707/114
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FEP94]
[FEP94]	(Forbes+Elson+Phillips+, 1994)
Write:	<<[FEP94] NNN>>
N:	203
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	observations from HST WFC-II
Ref:	=1994ApJ...437L..17F
by	FORBES D.A. , ELSON R.A.W., PHILLIPS A.C., ILLINGWORTH G.D., KOO D.C.
	Astrophys. J., 437, 17-None (1994)
	The nuclear colors and morphology of field galaxies at moderate redshift.
o	Table 2: <[FEP94] NNN> N=203
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Fermi
Fermi	(Fermi Gamma Ray Space Telescope)
Write:	<<Fermi bnYYMMDDddd>>
Object:	(Gamma) (SIMBAD class: gammaBurst = Gamma-ray Burst)
Note:	Fermi GBM Trigger Catalog (triggers observed by one or more of the 14 GBM detectors). For more details, see http://heasarc.gsfc.nasa.gov/W3Browse/fermi/fermigtrig.html
Ref:	=2012ApJS..199...18P
by	PACIESAS W.S. , MEEGAN C.A., VON KIENLIN A., BHAT P.N., BISSALDI E., BRIGGS M.S., BURGESS J.M., CHAPLIN V., CONNAUGHTON V., DIEHL R., FISHMAN G.J., FITZPATRICK G., FOLEY S., GIBBY M., GILES M., GOLDSTEIN A., GREINER J., GRUBER D., GUIRIEC S., VAN DER HORST A.J., KIPPEN R.M., KOUVELIOTOU C., LICHTI G., LIN L., McBREEN S., PREECE R.D., RAU A., TIERNEY D., WILSON-HODGE C.
	Astrophys. J., Suppl. Ser., 199, 18 (2012)
	The Fermi GBM Gamma-Ray Burst catalog: the first two years.
o	Tables 2-5: <Fermi bnYYMMDDddd> N=492.
Ref:	=2014ApJS..211...13V
by	VON KIENLIN A. , MEEGAN C.A., PACIESAS W.S., BHAT P.N., BISSALDI E., BRIGGS M.S., BURGESS J.M., BYRNE D., CHAPLIN V., CLEVELAND W., CONNAUGHTON V., COLLAZZI A.C., FITZPATRICK G., FOLEY S., GIBBY M., GILES M., GOLDSTEIN A., GREINER J., GRUBER D., GUIRIEC S., VAN DER HORST A.J., KOUVELIOTOU C., LAYDEN E., McBREEN S., McGLYNN S., PELASSA V., PREECE R.D., RAU A., TIERNEY D., WILSON-HODGE C.A., XIONG S., YOUNES G., YU H.-F.
	Astrophys. J., Suppl. Ser., 211, 13 (2014)
	The second Fermi GBM γ-ray burst catalog: the first four years.
o	Tables 6-9: <Fermi bnYYMMDDddd> N=954.
o	In table 6, GRB 100724A is GRB 100724B (=bn100724029), GRB 120222A (for bn120222119) is GRB 120222B, GRB 101214A (for bn101214993) is GRB 101214B, GRB 110920A (for bn110920338) is GRB 110920B and GRB 110517A (for bn110517573) is GRB 110517B and GRB 110517B (for bn110517902) is GRB 110517C.
Ref:	=2016ApJS..223...28B
by	BHAT P.N. , MEEGAN C.A., VON KIENLIN A., PACIESAS W.S., BRIGGS M.S., BURGESS J.M., BURNS E., CHAPLIN V., CLEVELAND W.H., COLLAZZI A.C., CONNAUGHTON V., DIEKMANN A.M., FITZPATRICK G., GIBBY M.H., GILES M.M., GOLDSTEIN A.M., GREINER J., JENKE P.A., KIPPEN R.M., KOUVELIOTOU C., MAILYAN B., McBREEN S., PELASSA V., PREECE R.D., ROBERTS O.J., SPARKE L.S., STANBRO M., VERES P., WILSON-HODGE C.A., XIONG S., YOUNES G., YU H.-F., ZHANG B.
	Astrophys. J., Suppl. Ser., 223, 28-28 (2016)
	The third Fermi GBM γ-ray burst catalog: the first six years.
o	Tables 5-8: <Fermi bnYYMMDDddd> N=1405.
Ref:	=2020ApJ...893...46V
by	VON KIENLIN A. , MEEGAN C.A., PACIESAS W.S., BHAT P.N., BISSALDI E., BRIGGS M.S., BURNS E., CLEVELAND W.H., GIBBY M.H., GILES M.M., GOLDSTEIN A., HAMBURG R., HUI C.M., KOCEVSKI D., MAILYAN B., MALACARIA C., POOLAKKIL S., PREECE R.D., ROBERTS O.J., VERES P., WILSON-HODGE C.A.
	Astrophys. J., 893, 46-46 (2020)
	The fourth Fermi-GBM Gamma-ray Burst catalog: a decade of data.
o	Tables 4-7: <Fermi bnYYMMDDddd> N=2360.
=E=	Catalogue in electronic form as J/ApJS/199/18
=E=	Catalogue in electronic form as J/ApJS/211/13
=E=	Catalogue in electronic form as <J/ApJS/223/28/>
=E=	Catalogue in electronic form as <J/ApJ/893/46/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Fermi
Fermi	(Fermi Gamma Ray Space Telescope)
Write:	<<Fermi JHHMM+DDMM>> <<Fermi JHHMM.m+DDMM>>
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	Fermi Gamma-ray Space Telescope observations. Only the first encountered reference for each format is listed here.
Ref:	=2009ATel.2081....1Y
by	YASUDA H. , TAKAHASHI H., McCONVILLE W.
	ATel, 2081, 1-1 (2009)
	Fermi LAT detection of a new γ-ray transient in the galactic plane: J1057-6027.
o	<Fermi JHHMM+DDMM> N=1.
Ref:	=2013ATel.4949....1N
by	NISHIMICHI M. , MORI M.
	ATel, 4949, 1 (2013)
	Fermi LAT detection of two high Galactic latitude γ-ray sources, Fermi J1049.7+0435 and J1103.2+1145.
o	<Fermi JHHMM.m+DDMM> N=2.
Origin	of the Acronym: A = Assigned by the author(s)
History	of this Acronym: replaces [YTM2009],
Details on Acronym: Ferrero
Ferrero	(Ferrero)
Write:	<<Cl Ferrero NN>>
N:	3
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
=E=	Catalogue in electronic form as B/ocl
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FES2017]
[FES2017]	(Faifer+Escudero+Scalia+, 2017)
Write:	<<[FES2017] NGC 5044-UCD1>>
N:	1
Object:	UCD (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Gemini South GMOS observations of N=1 ultra compact dwarf galaxy in the NGC 5044 group of galaxies.
in source:	NAME NGC 5044 Group
Ref:	=2017A&A...599L...8F
by	FAIFER F.R. , ESCUDERO C.G., SCALIA M.C., SMITH CASTELLI A.V., NORRIS M., DE ROSSI M.E., FORTE J.C., CELLONE S.A.
	Astron. Astrophys., 599L, 8-8 (2017)
	First confirmed ultra-compact dwarf galaxy in the NGC 5044 group.
o	<[FES2017] NGC 5044-UCD1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FeSt
FeSt	(Feitzinger+Stuve)= (FS)
Write:	<<FeSt 1-NNN>> <<FeSt 2-NNN>>
N:	489+331
Object:	Dark Cloud + Globule (SIMBAD class: ISM = Interstellar Medium Object)
Stat:	is completely incorporated in Simbad
Note:	List 1: format '1-NNN', N=489 DCld. List 2: format '2-NNN:, N=331 Globules.
Ref:	=1984A&AS...58..365F
by	FEITZINGER J.V. , STUWE J.A.
	Astron. Astrophys., Suppl. Ser., 58, 365-386 (1984)
	Catalogue of dark nebulae and globules for galactic longitudes 240 to 360 °.
o	(Erratum) Erratum 1986, A+AS vol. 63, p. 203
o	DkCloud: <FeSt 1-NNN> (Nos 1-1 to 1-489). Globules: <FeSt 2-NNN> (Nos 2-1 to 2-331).
=E=	Catalogue in electronic form as VII/68
Details on Acronym: FF
FF	(FIRST+FSC)
Write:	<<FF JHHMM+DDMM>>
N:	108+28
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	New sample of distant ultraluminous IR galaxies. The sample was selected from a positional cross-correlation of the IRAS Faint Source Catalog (FSC) with the FIRST database. Optical finding charts.
Ref:	=2000ApJS..131..185S
by	STANFORD S.A. , STERN D., VAN BREUGEL W., DE BREUCK C.
	Astrophys. J., Suppl. Ser., 131, 185-221 (2000)
	The FIRST sample of ultraluminous infrared galaxies at high redshift. I. Sample and near-infrared morphologies.
o	Table 1: <FF JHHMM+DDMM> N=108.
Ref:	=2006AJ....131.2877L
by	LAAG E.A. , CANALIZO G., VAN BREUGEL W., GATES E.L., DE VRIES W., STANFORD S.A.
	Astron. J., 131, 2877-2887 (2006)
	Adaptive optics imaging survey of luminous infrared galaxies.
o	Table 1: <FF JHHMM+DDMM> N=28 added.
=E=	Catalogue in electronic form as J/ApJS/131/185
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FF93]
[FF93]	(Flynn+Freeman, 1993)
Write:	<<[FF93] 5NNNNN>>
N:	128
Object:	K Giant (SIMBAD class: Star)
Note:	Format is always with 6 digits, the first digit been always a '5'
Ref:	=1993A&AS...97..835F
by	FLYNN C. , FREEMAN K.C.
	Astron. Astrophys., Suppl. Ser., 97, 835-849 (1993)
	A catalog of K giants at the South Galactic Pole: broad band and DDO photometry and radial velocities.
o	<[FF93] 5NNNNN> N=128.
=E=	Catalogue in electronic form as J/A+AS/97/835
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFD2016]
[FFD2016]	(Farina+Fumagalli+Decarli+, 2016)
Write:	<<[FFD2016] NN>>
N:	18
Object:	G (SIMBAD class: Galaxy)
Note:	Baade Magellan 6.5m telescope IMACS multi-object spectroscopic observations of N=17 galaxies the field of PKS 2155-304. See also [FGM91] and <%M [PWC2011].
in source:	PKS 2155-304
Ref:	=2016MNRAS.455..618F
by	FARINA E.P. , FUMAGALLI M., DECARLI R., FANIDAKIS N.
	Mon. Not. R. Astron. Soc., 455, 618-625 (2016)
	The cluster-scale environment of PKS 2155-304.
o	Tables 1-2: <[FFD2016] NN> N=18 among (Nos 8-29), <[FFD2016] Neb> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFF2004]
[FFF2004]	(Forbes+Faifer+Forte+, 2004)
Write:	<<[FFF2004] xxxx-yyyy>>
N:	2151
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Sloan g and i imaging from the Gemini Multi-Object Spectrograph (GMOS) instrument on the Gemini North telescope. Among the 2151 identified extended objects observed, 995 are candidate globular clusters.
in source:	M 60 = NGC 4649
Ref:	=2004MNRAS.355..608F
by	FORBES D.A. , FAIFER F.R., FORTE J.C., BRIDGES T., BEASLEY M.A., GEBHARDT K., HANES D.A., SHARPLES R., ZEPF S.E.
	Mon. Not. R. Astron. Soc., 355, 608-616 (2004)
	Gemini/GMOS imaging of globular clusters in the Virgo galaxy NGC 4649 (M60).
o	Tables 1, A1: <[FFF2004] XXXX-YYYY> N=2151.
=E=	Catalogue in electronic form as J/MNRAS/355/608
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFF98]
[FFF98]	(Fisher+Fabricant+Franx+, 1998)
Write:	<<[FFF98] NNNN>>
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Finding charts. See also [KVF97], [FMB91], [FFV2000].
in source:	ClG 1358+6245 = 1E 1358.4+6245
Ref:	=1998ApJ...498..195F
by	FISHER D. , FABRICANT D., FRANX M., VAN DOKKUM P.
	Astrophys. J., 498, 195-212 (1998)
	A spectroscopic survey of the galaxy cluster CL 1358+62 at z = 0.328.
o	Table 1: <[FFF98] NNNN> N=232 among (Nos 5-2081)
Ref:	=1998ApJ...500..714V
by	VAN DOKKUM P.G. , FRANX M., KELSON D.D., ILLINGWORTH G.D., FISHER D., FABRICANT D.
	Astrophys. J., 500, 714-737 (1998)
	The color-magnitude relation in CL 1358+62 at z = 0.33: evidence for significant evolution in the S0 population.
o	Table 1: <[FFF98] NNNN> N=194 among (Nos 86-1978)
=E=	Catalogue in electronic form as J/ApJ/498/195
=E=	Catalogue in electronic form as J/ApJ/500/714
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFG2001]
[FFG2001]	(Feretti+Fusco-Femiano+Giovannini+, 2001)
Write:	<<[FFG2001] DN>> <<[FFG2001] TN>> <<[FFG2001] JHHMM+DDd>> <<[FFG2001] JHHMMSS.s+DDMMSS>>
N:	4+3+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Study of ACO 2163. Fig.2: (Nos D1-D4), N=4 diffuse feature at the periphery of ACO 2163. Fig.2, Table 3: (Nos T1-T3), N=3 radio-sources showing a tailed structure, and coincident with faint G format 'JHHMM+DDd'. Text: 'J161622.2-060634' is a strong radio coincident with faint G.
in source:	ACO 2163
Ref:	=2001A&A...373..106F
by	FERETTI L. , FUSCO-FEMIANO R., GIOVANNINI G., GOVONI F.
	Astron. Astrophys., 373, 106-112 (2001)
	The giant radio halo in Abell 2163.
o	Fig.2: <[FFG2001] DN> (Nos D1-D4). Fig.2, Table 3: <[FFG2001] TN> (Nos T1-T3) = <[FFG2001] JHHMM+DDd> N=3. p.107: <[FFG2001] JHHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFG2007]
[FFG2007]	(Forte+Faifer+Geisler, 2007)
Write:	<<[FFG2007] NGC 1399 NNNNN>> <<[FFG2007] NGC 4486 NNNNNN>>
N:	6825+8477
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	KPNO Mayall and CTIO Blanco-4m telescope observations of NGC 1399 and NGC 4486 (M87).
in source:	NGC 1399
in source:	NGC 4486 = M 87
Ref:	=2007MNRAS.382.1947F
by	FORTE J.C. , FAIFER F., GEISLER D.
	Mon. Not. R. Astron. Soc., 382, 1947-1964 (2007)
	A quantitative link between globular clusters and the stellar haloes in elliptical galaxies.
o	Table 1: <[FFG2007] NGC 1399 NNNNN> N=6825. Table 2: <[FFG2007] NGC 4486 NNNNNN> N=8477.
=E=	Catalogue in electronic form as J/MNRAS/382/1947
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFH2002]
[FFH2002]	(Fadda+Flores+Hasinger+, 2002)
Write:	<<[FFH2002] NNN>>
N:	24
Object:	AGN (SIMBAD class: AGN = Active Galaxy Nucleus)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton sources in the Lockman Hole.
in source:	NAME Lockman Hole
Ref:	=2002A&A...383..838F
by	FADDA D. , FLORES H., HASINGER G., FRANCESCHINI A., ALTIERI B., CESARSKY C.J., ELBAZ D., FERRANDO P.
	Astron. Astrophys., 383, 838-853 (2002)
	The AGN contribution to mid-infrared surveys. X-ray counterparts of the mid-IR sources in the Lockman Hole and HDF-N.
o	Table 3, col(1): <[FFH2002] NNN> N=24 among (Nos 1-121). Table 3, col(2): <RDS NNNA> (Nos 438A, 814A) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFH96]
[FFH96]	(Ferrarese+Freedman+Hill+, 1996)
Write:	<<[FFH96] CNN>> <<[FFH96] N1>>
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations. Table 3A: N=70 Cepheids, (Nos C1-C70). N=1 Nova, No. N1. Preliminary results in 1994Natur.371..757F. See also: [FHM94], [HST94], [KIF96], [SHM96], [GPF97], [RMM97], [PSF98], [FBK98], [HHH98], [TFS98], [GHS99], [KIS99], [SHF99], [GFF99], [MHS99], [SFK99], [PKB99], [GSF2000], [MHS2000]
in source:	M 100 = NGC 4321
Ref:	=1996ApJ...464..568F
by	FERRARESE L. , FREEDMAN W.L., HILL R.J., SAHA A., MADORE B.F., KENNICUTT R.C.Jr, STETSON P.B., FORD H.C., GRAHAM J.A., HOESSEL J.G., HAN M., HUCHRA J., HUGHES S.M., ILLINGWORTH G.D., KELSON D., MOULD J.R., PHELPS R., SILBERMANN N.A., SAKAI S., TURNER A., HARDING P., BRESOLIN F.
	Astrophys. J., 464, 568-599 (1996)
	The extragalactic distance scale key project. IV. The discovery of Cepheids and a new distance to M100 using the Hubble Space Telescope.
o	(Erratum) erratum vol. 475, p. 853
o	Table 3A: <[FFH96] CNN> (Nos C1-C70), <[FFH96] N1> No. N1, N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFL2006]
[FFL2006]	(Forster Schreiber+Franx+Labbe+, 2006)
Write:	<<[FFL2006] NNNN>>
N:	1858
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	VLT ISAAC NIR observations of the field of 1E 1054.4-0321 as part of the FIRES.
in source:	1E 1054.4-0321 = ClG 1054-0321
Ref:	=2006AJ....131.1891F
by	FOERSTER-SCHREIBER N.M. , FRANX M., LABBE I., RUDNICK G., VAN DOKKUM P.G., ILLINGWORTH G.D., KUIJKEN K., MOORWOOD A.F.M., RIX H.-W., ROETTGERING H., VAN DER WERF P.
	Astron. J., 131, 1891-1913 (2006)
	Faint infrared extragalactic survey: data and source catalog of the MS 1054-03 field.
o	Catalog: <[FFL2006] NNNN> (Nos 1-1858).
=E=	Catalogue in electronic form as J/AJ/131/1891
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFL2007]
[FFL2007]	(Faria+Feltzing+Lundstrom+, 2007)
Write:	<<[FFL2007] NNNN>>
N:	180
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	INT Wide Field Camera (WFC) observations of the Draco galaxy.
in source:	NAME Draco Dwarf Galaxy
Ref:	=2007A&A...465..357F
by	FARIA D. , FELTZING S., LUNDSTROEM I., GILMORE G., WAHLGREN G.M., ARDEBERG A., LINDE P.
	Astron. Astrophys., 465, 357-373 (2007)
	The usage of Stroemgren photometry in studies of local group dwarf spheroidal galaxies. Application to Draco: a new catalogue of Draco members and a study of the metallicity distribution function and radial gradients.
o	Tables 4, 6, Figs.: <[FFL2007] NNNN> N=119+5+4+2 among (Nos 53-3233).
=E=	Catalogue in electronic form as J/A+A/465/357
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFM2004]
[FFM2004]	(Filho+Fraterlani+Markoff+, 2004)
Write:	<<[FFM2004] NGC 5846 A>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLBA observations. Maps of NGC 5846 show a multiple radio-source.
in source:	NGC 5846
Ref:	=2004A&A...418..429F
by	FILHO M.E. , FRATERNALI F., MARKOFF S., NAGAR N.M., BARTHEL P.D., HO L.C., YUAN F.
	Astron. Astrophys., 418, 429-443 (2004)
	Further clues to the nature of composite LINER/H II galaxies.
o	Table 2, Fig.2: <[FFM2004] NGC 5846 A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFN2011]
[FFN2011]	(Faifer+Forte+Norris+, 2011)
Write:	<<[FFN2011] NNNNN GC NNNN>> <<[FFN2011] NNNNN GC R NNNNNN>> <<[FFN2011] NNNNN UCD NNNN>> <<[FFN2011] NNNNN UCD R NNNNNN>>
N:	3345+75
Object:	Poss. GlCl + Poss. UCD (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	Gemini North and South g'r'i' photometry of globular cluster and ultra compact dwarf candidates in five early-type galaxies.
in source:	NGC 4649
in source:	NGC 3923
in source:	NGC 524
in source:	NGC 3115
in source:	NGC 3379
Ref:	=2011MNRAS.416..155F
by	FAIFER F.R. , FORTE J.C., NORRIS M.A., BRIDGES T., FORBES D.A., ZEPF S.E., BEASLEY M., GEBHARDT K., HANES D.A., SHARPLES R.M.
	Mon. Not. R. Astron. Soc., 416, 155-177 (2011)
	Gemini/GMOS imaging of globular cluster systems in five early-type galaxies.
o	Table A1: <[FFN2011] NNNNN GC NNNN>, <[FFN2011] NNNNN GC R NNNNNN>, N=3345. Table A2: <[FFN2011] NNNNN UCD NNNN>, <[FFN2011] NNNNN UCD R NNNN>, N=75.
=E=	Catalogue in electronic form as <J/MNRAS/416/155/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFO2009]
[FFO2009]	(Faundez-Abans+Fernandes+De Oliveira-Abans+, 2009)
Write:	<<[FFO2009] a>> <<[FFO2009] F>> <<[FFO2009] WW>>
N:	3+1+2
Object:	G + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Observations of the field of HRG 54103 with the 1.6m telescope at the Observatorio do Pico dos Dias and the CTIO 1.5m telescope.
Ref:	=2009A&A...507.1303F
by	FAUNDEZ-ABANS M. , FERNANDES I.F., DE OLIVEIRA-ABANS M., POPPE P.C.R., MARTIN V.A.F.
	Astron. Astrophys., 507, 1303-1311 (2009)
	The ring galaxy HRG 54103: a first study.
o	Fig. 1: <[FFO2009] a> (Nos a-c), <[FFO2009] F> N=1, <[FFO2009] WW> (Nos S, SE).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFP2005]
[FFP2005]	(Fugazza+Fiore+Patat+, 2005)
Write:	<<[FFP2005] GRB 050908 abs N.NNN>>
N:	1
Object:	Absorber
Note:	VLT FORS observations. Host galaxy of GRB 050908.
Ref:	=2005GCN..3948....1F
by	FUGAZZA D. , FIORE F., PATAT N., LEDOUX C., D'AVANZO P., ANTONELLI L.A., CHINCARINI G., MALESANI D., COVINO S., TAGLIAFERRI G., PIRANOMONTE S., STELLA L.
	GRB Coordinates Network, Circular Service, 3948, 1-None (2005)
	GRB 050908: spectroscopic redshift.
o	<[FFP2005] GRB 050908 abs N.NNN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFP89]
[FFP89]	(Fanti+Fanti+Parma+, 1989)
Write:	<<[FFP89] 3C NNN A>>
N:	3+4+7
Object:	Component (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Morphologies of 3 radio-sources.
in source:	3C 49
in source:	3C 138
in source:	3C 287
Ref:	=1989A&A...217...44F
by	FANTI C. , FANTI R., PARMA P., VENTURI T., SCHILIZZI R.T., NAN R.-D., SPENCER R.E., MUXLOW T.W.B., VAN BREUGEL W.
	Astron. Astrophys., 217, 44-56 (1989)
	Three prototype compact steep spectrum radio sources.
o	Table 3, Fig.3: <[FFP89] 3C 287 A> (Nos A-C). Table 4, Fig.4: <[FFP89] 3C 49 A> (Nos A-D). Table 5, Fig.7: <[FFP89] 3C 138 A> (Nos A-G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFP95]
[FFP95]	(Feretti+Fanti+Parma+, 1995)
Write:	<<[FFP95] 1615+35 A>> <<[FFP95] 1615+35 AN>> <<[FFP95] 1621+38 A>>
N:	2+4+5
Object:	(Rad) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Table 3: N=6 obj. in the field 1615+35, format '1615+35 A' or '1615+35 AN', Nos A1-A2, B1-B2, C, D. Table 4: N=5 obj. in the field 1621+38, format '1621+38 A', (Nos A-E)
Ref:	=1995A&A...298..699F
by	FERETTI L. , FANTI R., PARMA P., MASSAGLIA S., TRUSSONI E., BRINKMANN W.
	Astron. Astrophys., 298, 699-710 (1995)
	ROSAT observations of the B2 radio galaxies 1615+35 and 1621+38: implications for the radio source confinement.
o	Table 3: <[FFP95] 1615+35 A> or <[FFP95] 1615+35 AN> Nos A1-A2, B1-B2, C, D. Table 4: <[FFP95] 1621+38 A> (Nos A-E)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFS84]
[FFS84]	(Ftaclas+Fanelli+Struble, 1984)
Write:	<<[FFS84] Cloud A>>
N:	2
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Structure of the Virgo cluster region. The designation 'Cloud' is used for group of galaxies, and often found in literature as 'M Cloud' instead of 'Cloud M'. Cloud M and Cloud N are 2 subgroups in the field of the Virgo cluster. See also [D61], BTS87.
in source:	NAME Virgo Cluster
Ref:	=1984ApJ...282...19F
by	FTACLAS C. , FANELLI M.N., STRUBLE M.F.
	Astrophys. J., 282, 19-28 (1984)
	Velocity distribution of Virgo cluster galaxies.
o	12 12.5 +13 45
o	Fig.10: <[FFS84] Cloud A> (Nos M, N>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFS86]
[FFS86]	(Fanti+Fanti+Schilizzi+, 1986)
Write:	<<[FFS86] 3C 119 A>>
N:	7
Object:	Component (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Morphology of 3C 119. See also [NSV91] where the numbering is different.
in source:	3C 119
Ref:	=1986A&A...170...10F
by	FANTI C. , FANTI R., SCHILIZZI R.T., SPENCER R.E., VAN BREUGEL W.J.M.
	Astron. Astrophys., 170, 10-19 (1986)
	The peculiar morphology of the compact steep spectrum radio source 3C 119.
o	Figs 2, Table 2: <[FFS86] 3C 119 A> (Nos A-G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFT2015]
[FFT2015]	(Finkelstein+Finkelstein+Tilvi+, 2015)
Write:	<<[FFT2015] NNc>> <<[FFT2015] NNNnc>>
N:	61+14
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC observations of N=75 Lyα emitting galaxies (LAEs) in the Bootes field at z~5.5 and z~5.7. In the format "c" stands for spectroscopically confirmed LAEs and "nc" stands for not spectroscopically confirmed LAEs. Use of archival Spitzer Lyα survey and HST NICMOS and WFC3 images.
in source:	NAME Bootes Field
Ref:	=2015ApJ...813...78F
by	FINKELSTEIN K.D. , FINKELSTEIN S.L., TILVI V., MALHOTRA S., RHOADS J.E., GROGIN N.A., PIRZKAL N., DEY A., JANNUZI B.T., MOBASHER B., PAKZAD S., SALMON B., WANG J.
	Astrophys. J., 813, 78 (2015)
	Probing the physical properties of z = 4.5 Lyman α emitters with Spitzer.
o	Table 2: <[FFT2015] NNc> N=30 among (Nos 3c-56c), <[FFT2015] NNnc> N=31 among (Nos 10nc-196nc). Table 3: <[FFT2015] NNc> N=5 among (Nos 54c-63c), <[FFT2015] NNNnc> N=9 among (Nos 202nc-231nc).
=E=	Catalogue in electronic form as J/ApJ/813/78
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFV2000]
[FFV2000]	(Fabricant+Franx+Van Dokkum+, 2000)
Write:	<<[FFV2000] NNNN>>
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	HST WFPC2 observations. Photometric catalog of N=518 galaxies in ClG 1358+62. See also [KVF97], [FFF98], [FMB91]
in source:	ClG 1358+6245 = 1E 1358.4+6245
Ref:	=2000ApJ...539..577F
by	FABRICANT D. , FRANX M., VAN DOKKUM P.
	Astrophys. J., 539, 577-591 (2000)
	Galaxy morphologies in the cluster Cl 1358+62 at z=0.33.
o	Table 2: <[FFV2000] NNNN> N=298 among (Nos 1-1666).
=E=	Catalogue in electronic form as J/ApJ/539/577
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FFV2013]
[FFV2013]	(Forte+Faifer+Vega+, 2013)
Write:	<<[FFV2013] DDD.ddddddd+DD.ddddddd>>
N:	338
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	Gemini North GMOS observations of N=338 globular cluster candidates in the field of M 87.
in source:	M 87 = NGC 4486 = Virgo A
Ref:	=2013MNRAS.431.1405F
by	FORTE J.C. , FAIFER F.R., VEGA E.I., BASSINO L.P., SMITH CASTELLI A.V., CELLONE S.A., GEISLER D.
	Mon. Not. R. Astron. Soc., 431, 1405-1416 (2013)
	Multicolour-metallicity relations from globular clusters in NGC 4486 (M87).
o	Table 4: <[FFV2013] DDD.ddddddd+DD.ddddddd> N=338.
=E=	Catalogue in electronic form as J/MNRAS/431/1405
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FG
FG	(Falgarone+Gilmore)
Write:	<<FG LNNNN NN>> <<FG Tau NN>> <<FG Oph NN>> <<FG S140 NN>>
N:	13+15+13+27+29
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	HII in LDN 1471: format 'L1471 NN', N=13. HII in Taurus: format 'Tau NN', N=13. HII in LDN 1547: format 'L1547 NN', N=15. HII in ρ Oph: format 'Oph NN', N=27. HII in Sh 2-140 IR: format 'S140 NN', N=29.
in source:	LDN 1471
in source:	LDN 1547
in source:	NAME TMC
in source:	NAME rho Oph Cloud
in source:	SH 2-140
Ref:	=1981A&A....95...32F
by	FALGARONE E. , GILMORE W.
	Astron. Astrophys., 95, 32-38 (1981)
	Partial aperture synthesis of five dark clouds at 1.4 GHz.
o	<FG L1471 NN> N=13, <FG Tau NN> N=13, <FG L1547 NN> N=15, <FG Oph NN> N=27, <FG S140 NN> N=29
Origin	of the Acronym: L = Found in the literature
Details on Acronym: FG
FG	(Feitzinger+Galinski)
*****	Avoid the usage of FG, prefer [FG85]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Fg
Fg	(Fleming)= (Fl) = (Fleming)
Write:	<<PN Fg N>>
N:	3
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	3 PN excerpted from a list of 31 objects. Fg 1 = PN G290.5+07.9 = PK 290+07 1. Fg 2 = PN G346.3-06.8 = PK 346-06 1. Fg 3 = PN G352.9-07.5 = PK 352-07 1
Ref:	=1910HarCi.158....0F
by	FLEMING M.
	Harvard Circ., -1-None (1910)
	Stars having peculiar spectra. 38 new variables stars.
Ref:	=1911HarCi.167....0F
by	FLEMING M.
	Harvard Circ., -1-None (1911)
	Stars having peculiar spectra. 31 new variables stars.
Details on Acronym: [FG2000]
[FG2000]	(Fruchter+Goss, 2000)= ([FG2000a])
Write:	<<[FG2000] Terzan 5 W>> <<[FG2000] Terzan 5 W'>> <<[FG2000] Terzan 5 A>> <<[FG2000] JHHMMSS.ss+DDMMSS.s>> <<[FG2000] 47 Tuc N>> <<[FG2000] 47 Tuc A>>
N:	4+3+3+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA observations of globular clusters. Table 1: N=5 sources in Terzan 5, (Nos N, S, N', C). Table 2: N=1 source 'JHHMMSS.ss+DDMMSS.s' in NGC 6539, N=1 in NGC 6624, N=1 in NGC 6440. Table 3: N=5 sources in 47 Tuc, (Nos C, D, 1-3). Table 4: N=1 source 'JHHMMSS.ss+DDMMSS.s' in Liller 1.
in source:	Cl Terzan 5
in source:	NGC 6539
in source:	NGC 6624
in source:	NGC 6440
in source:	NGC 104 = 47 Tuc
in source:	Liller 1
Ref:	=2000ApJ...536..865F
by	FRUCHTER A.S. , GOSS W.M.
	Astrophys. J., 536, 865-874 (2000)
	Deep radio imaging of globular clusters and the cluster pulsar population.
o	(Erratum) Erratum vol. 551, p. 597 (2001)
o	Table 3: 47 Tuc C and D = PSR J0024-72C and PSR J0024-72D.
o	Table 1: <[FG2000] Terzan 5 W> (Nos N, S), <[FG2000] Terzan 5 W'> (No. N'), <[FG2000] Terzan 5 A> (No. C). Tables 2, 4: <[FG2000] JHHMMSS.ss+DDMMSS.s> N=4. Table 3: <[FG2000] 47 Tuc N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FG2000a]
[FG2000a]	(Fruchter+Goss, 2000)
*****	Avoid the usage of [FG2000a], prefer [FG2000]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FG2000b]
[FG2000b]	(Fassett+Graham, 2000)
Write:	<<[FG2000b] NN>>
N:	50
Object:	* (SIMBAD class: Star)
Note:	HST WFPC2 archival data. Table 3: N=50 brightest blue stars in the field of Cen A. See also [MRG2000].
in source:	Cen A = NGC 5128
Ref:	=2000ApJ...538..594F
by	FASSETT C.I. , GRAHAM J.A.
	Astrophys. J., 538, 594-607 (2000)
	Age, evolution, and dispersion of the loose groups of blue stars in the northeast radio lobe of Centaurus A.
o	Table 1: [ZHG90b] NGC 5128 NN
o	Table 3: <[FG2000b] NN> (Nos 1-50).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FG85]
[FG85]	(Feitzinger+Galinski, 1985)= (FG)
Write:	<<[FG85] NNN>>
N:	584
Object:	Dwarf G (SIMBAD class: Galaxy)
Ref:	=1985A&AS...61..503F
by	FEITZINGER J.V. , GALINSKI T.
	Astron. Astrophys., Suppl. Ser., 61, 503-515 (1985)
	A catalogue of dwarf galaxies south of δ = -17 5.
o	<[FG85] NNN> (Nos 1-584)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FG93]
[FG93]	(Lauer+Fber, 1993) (Not yet in Simbad)
Write:	<<[FG93] PN>>
N:	2
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=2 peaks in the nucleus of M 31
in source:	M 31 = NGC 224
Ref:	=1993AJ....106.1436L
by	LAUER T.R. , FABER S.M., GROTH E.J., SHAYA E.J., CAMPBELL B., CODE A., CURRIE D.G., BAUM W.A., EWALD S.P., HESTER J.J., HOLTZMAN J.A., KRISTIAN J., LIGHT R.M., LIGYNDS C.R., O'NEIL E.J.Jr, WESTPHAL J.A.
	Astron. J., 106, 1436-1447 (1993)
	Planetary camera observations of the double nucleus of M 31.
o	<[LFG93] PN> (Nos P1-P2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FG96]
[FG96]	(Fesen+Gunderson, 1996)
Write:	<<[FG96] NNA>>
N:	87+43
Object:	Knot (SIMBAD class: PartofCloud = Part of Cloud)
Note:	(Nos 1-87) knots in Cas A SNR. In the 2nd ref., format 'NNA' is used for the newly discoveed knots, identified with an already known nearby knot and adding a letter (e.g. knot 3 and 3A-3B, 19 and 19A-19M) Identif. chart in Fig. 3 in 1st ref. Identif. chart in Fig. 1 and finding charts in Figs 2 in 2nd ref. See also [HG96] and [FHM2006].
in source:	NAME Cas A
Ref:	=1996ApJ...470..967F
by	FESEN R.A. , GUNDERSON K.S.
	Astrophys. J., 470, 967-980 (1996)
	Optical spectroscopy and imaging of the northeast jet in the Cassiopeia A supernova remnant.
o	cross-id. Number NNN in FBG = KB MK NNN', Minkovski ('M NN') not in SIMBAD
o	Tables 1-11: <[FG96] NN> (Nos 1-87)
Ref:	=2001ApJS..133..161F
by	FESEN R.A.
	Astrophys. J., Suppl. Ser., 133, 161-186 (2001)
	An optical survey of outlying ejecta in Cassiopeia A: evidence for a turbulent, asymmetric explosion.
o	Tables 2, 3, 4: <[FG96] NNA> N=43 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FGB2009]
[FGB2009]	(Forster Schreiber+Genzel+Bouche+, 2009) (Not yet in Simbad)
Write:	<<[FGB2009] GMASS 2113W>> <<[FGB2009] GDDS SA12-8768NW>>
N:	2+1
Object:	G (SIMBAD class: Galaxy)
Note:	VLT SINFONI observations of faint companions to GMASS 2113 and GDDS SA12-8768.
Ref:	=2009ApJ...706.1364F
by	FORSTER SCHREIBER N.M. , GENZEL R., BOUCHE N., CRESCI G., DAVIES R., BUSCHKAMP P., SHAPIRO K., TACCONI L.J., HICKS E.K.S., GENEL S., SHAPLEY A.E., ERB D.K., STEIDEL C.C., LUTZ D., EISENHAUER F., GILLESSEN S., STERNBERG A., RENZINI A., CIMATTI A., DADDI E., KURK J., LILLY S., KONG X., LEHNERT M.D., NESVADBA N., VERMA A., McCRACKEN H., ARIMOTO N., MIGNOLI M., ONODERA M.
	Astrophys. J., 706, 1364-1428 (2009)
	The SINS survey: SINFONI integral field spectroscopy of z ~ 2 star-forming galaxies.
o	<[FGB2009] GMASS 2113W> (Nos E, W). <[FGB2009] GGDS SA12-8768NW> N=1.
=E=	Catalogue in electronic form as <J/ApJ/706/1364/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FGB97]
[FGB97]	(Feretti+Giovannini+Bohringer, 1997)
Write:	<<[FGB97] JHHMM+DDMMA>> <<[FGB97] A>>
N:	15
Object:	Radio G (SIMBAD class: RadioG = Radio Galaxy)
Note:	Table 4: N=15 radio galaxies, format 'JHHMM+DDMMA', cross-id. with a format 'A' as found in Fig.1. Radio maps in Fig.4
in source:	ACO 2319
Ref:	=1997NewA....2..501F
by	FERETTI L. , GIOVANNINI G., BOHRINGER H.
	New Astronomy, 2, 501-515 (1997)
	The radio and X-ray properties of Abell 2319.
o	cross-id. WSTB 13W, [OHF95] ACO 2319, [FD77] ACO 2319
o	Table 4: <[FGB97] JHHMM+DDMMA> N=15 and col(8): = <[FGB97] A> N=15 among (Nos A-S).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FGC
FGC	(Flat Galaxy Catalogue)
Write:	<<FGC NNNN>>
N:	2573
Object:	Spiral G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Beware: the headers of the col. are everywhere FGC, while p. 106-172 refer to FGC, p. 173-218 refer to FGCE, p. 219-222 refer to FGCA which is given the format 'NNNA'. See also RFGC.
Ref:	=1993AN....314...97K
by	KARACHENTSEV I.D. , KARACHENTSEVA V.E., PARNOVSKY S.L.
	Astron. Nachr., 314, 97-222 (1993)
	Flat galaxies catalogue.
o	(Erratum) erratum vol. 315, 264
o	<FGC NNNN> (Nos 1-2573), <FGCA NNNA> (Nos 1-A-291A), <FGCE NNNN> (Nos 1-1882).
=E=	Catalogue in electronic form as VII/162
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FGC2019]
[FGC2019]	(Forbes+Gannon+Couch+, 2019)
Write:	<<[FGC2019] NGC 5846 UDG1>> <<[FGC2019] NGC 5846 GCNN>>
N:	1+20
Object:	Ultra-diffuse G + Poss. GlCl (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	VST OmegaCAM observations of N=1 ultra diffuse galaxy (UDG) and N=20 globular cluster candidates in the NGC 5846 group. Use of VST survey of Early-type GAlaxieS (VEGAS) imaging.
in source:	NAME NGC 5846 GROUP
Ref:	=2019A&A...626A..66F
by	FORBES D.A. , GANNON J., COUCH W.J., IODICE E., SPAVONE M., CANTIELLO M., NAPOLITANO N., SCHIPANI P.
	Astron. Astrophys., 626A, 66-66 (2019)
	An ultra diffuse galaxy in the NGC 5846 group from the VEGAS survey.
o	Fig. 1, Table 1: <[FGC2019] NGC 5846 UDG1> N=1. Table 2: <[FGC2019] NGC 5846 GCNN> (Nos GC1-GC20).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FGCA
FGCA	(Flat Galaxy Catalogue, Addendum)
Write:	<<FGCA NNNA>>
N:	291
Object:	Spiral G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	In the format, 'A' for Addendum. See also FGC, FGCE, RFGC.
Ref:	=1993AN....314...97K
by	KARACHENTSEV I.D. , KARACHENTSEVA V.E., PARNOVSKY S.L.
	Astron. Nachr., 314, 97-222 (1993)
	Flat galaxies catalogue.
o	(Erratum) erratum vol. 315, 264
o	<FGC NNNN> (Nos 1-2573), <FGCA NNNA> (Nos 1-A-291A), <FGCE NNNN> (Nos 1-1882).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FGCE
FGCE	(Flat Galaxy Catalogue, southern Extension)
Write:	<<FGCE NNNN>>
N:	1882
Object:	Spiral G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Dec < -17.5deg. The letter 'E' is often added at the end of the format. See also FGC, FGCA, RFGC.
Ref:	=1993AN....314...97K
by	KARACHENTSEV I.D. , KARACHENTSEVA V.E., PARNOVSKY S.L.
	Astron. Nachr., 314, 97-222 (1993)
	Flat galaxies catalogue.
o	(Erratum) erratum vol. 315, 264
o	<FGC NNNN> (Nos 1-2573), <FGCA NNNA> (Nos 1-A-291A), <FGCE NNNN> (Nos 1-1882).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FGD2001]
[FGD2001]	(Fynbo+Gorosabel+Dall+, 2001)
Write:	<<[FGD2001] GRB 000926 Host G>> <<[FGD2001] Star A>>
N:	1+4
Object:	G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Finding chart of the field of GRB 000926. See also [CDK2000].
Ref:	=2001A&A...373..796F
by	FYNBO J.U. , GOROSABEL J., DALL T.H., HJORTH J., PEDERSEN H., ANDERSEN M.I., MOLLER P., HOLLAND S., SMAIL I., KOBAYASHI N., ROL E., VREESWIJK P., BURUD I., JENSEN B.L., THOMSEN B., HENDEN A., VRBA F., CANZIAN B., CASTRO CERON J.M., CASTRO-TIRADO A.J., CLINE T., GOTO M., GREINER J., HANSKI M.T., HURLEY K., LUND N., PURSIMO T., OSTENSEN R., SOLHEIM J., TANVIR N., TERADA H.
	Astron. Astrophys., 373, 796-804 (2001)
	The optical afterglow and host galaxy of GRB 000926.
o	Text: <[FGD2001] GRB 000926 Host G> N=1. Table 1: <[FGD2001] Star A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FGES
FGES	(Fermi Galactic Extended Source)
Write:	<<FGES JHHMM.m+DDMM>>
N:	46
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	The Fermi Galactic Extended Source Catalog contains N=46 extended sources from Fermi-Large Area Telescope (LAT) Pass 8 data.
Ref:	=2017ApJ...843..139A
by	ACKERMANN M. , AJELLO M., BALDINI L., BALLET J., BARBIELLINI G., BASTIERI D., BELLAZZINI R., BISSALDI E., BLOOM E.D., BONINO R., BOTTACINI E., BRANDT T.J., BREGEON J., BRUEL P., BUEHLER R., CAMERON R.A., CARAGIULO M., CARAVEO P.A., CASTRO D., CAVAZZUTI E., CECCHI C., CHARLES E., CHEKHTMAN A., CHEUNG C.C., CHIARO G., CIPRINI S., COHEN J.M., COSTANTIN D., COSTANZA F., CUTINI S., D'AMMANDO F., DE PALMA F., DESIANTE R., DIGEL S.W., DI LALLA N., DI MAURO M., DI VENERE L., FAVUZZI C., FEGAN S.J., FERRARA E.C., FRANCKOWIAK A., FUKAZAWA Y., FUNK S., FUSCO P., GARGANO F., GASPARRINI D., GIGLIETTO N., GIORDANO F., GIROLETTI M., GREEN D., GRENIER I.A., GRONDIN M.-H., GUILLEMOT L., GUIRIEC S., HARDING A.K., HAYS E., HEWITT J.W., HORAN D., HOU X., JOHANNESSON G., KAMAE T., KUSS M., LA MURA G., LARSSON S., LEMOINE-GOUMARD M., LI J., LONGO F., LOPARCO F., LUBRANO P., MAGILL J.D., MALDERA S., MALYSHEV D., MANFREDA A., MAZZIOTTA M.N., MICHELSON P.F., MITTHUMSIRI W., MIZUNO T., MONZANI M.E., MORSELLI A., MOSKALENKO I.V., NEGRO M., NUSS E., OHSUGI T., OMODEI N., ORIENTI M., ORLANDO E., ORMES J.F., PALIYA V.S., PANEQUE D., PERKINS J.S., PERSIC M., PESCE-ROLLINS M., PETROSIAN V., PIRON F., PORTER T.A., PRINCIPE G., RAINO S., RANDO R., RAZZANO M., RAZZAQUE S., REIMER A., REIMER O., REPOSEUR T., SGRO C., SIMONE D., SISKIND E.J., SPADA F., SPANDRE G., SPINELLI P., SUSON D.J., TAK D., THAYER J.B., THOMPSON D.J., TORRES D.F., TOSTI G., TROJA E., VIANELLO G., WOOD K.S., WOOD M.
	Astrophys. J., 843, 139-139 (2017)
	Search for extended sources in the galactic plane using six years of Fermi-Large Area Telescope Pass 8 data above 10 GeV.
o	Tables 1-3: <FGES JHHMM.m+DDMM> N=46.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FGF
FGF	(Franco+Garcia-Barreto+de la Fuente)
Write:	<<FGF NGC 1022 N>> <<FGF NGC 1326 N>> <<FGF NGC 4314 N>>
N:	3+1+3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio continuum emission sources in NGC 1022, NGC 1326, and NGC 4314. Maps in Figs 1, 3, 4.
in source:	NGC 1022
in source:	NGC 1326
in source:	NGC 4314
Ref:	=2000ApJ...544..277F
by	FRANCO J. , GARCIA-BARRETO J.A., DE LA FUENTE E.
	Astrophys. J., 544, 277-282 (2000)
	Decreasing density gradients in circumnuclear H II regions of barred galaxies NGC 1022, NGC 1326, and NGC 4314.
o	Table 1: <FGF NGC 1022 N> (Nos 1-3), <FGF NGC 1326 N> (No. 1), <FGF NGC 4314 N> (Nos 1-3).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FGG2015]
[FGG2015]	(Fang+Garcia-Benito+Guerrero+, 2015)
Write:	<<[FGG2015] PNNN>>
N:	7+11
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	GTC OSIRIS deep spectroscopy of N=7+11 planetary nebulae (PNe) in M31. See also [FZG2013].
in source:	M 31 = NGC 224
Ref:	=2015ApJ...815...69F
by	FANG X. , GARCIA-BENITO R., GUERRERO M.A., LIU X., YUAN H., ZHANG Y., ZHANG B.
	Astrophys. J., 815, 69 (2015)
	Chemical abundances of planetary nebulae in the substructures of M31.
o	Table 1: <[FGG2015] PNNN> (Nos PN1-PN7).
Ref:	=2018ApJ...853...50F
by	FANG X. , GARCIA-BENITO R., GUERRERO M.A., ZHANG Y., LIU X., MORISSET C., KARAKAS A.I., MILLER BERTOLAMI M.M., YUAN H., CABRERA-LAVERS A.
	Astrophys. J., 853, 50-50 (2018)
	Chemical abundances of planetary nebulae in the substructures of M31. II. The extended sample and a comparison study with the outer-disk group.
o	Table 1: <[FGG2015] PNNN> (Nos PN8-PN18) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FGH2007]
[FGH2007]	(Finoguenov+Guzzo+Hasinger+)
Write:	<<[FGH2007] NNN>>
N:	72
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	XMM-Newton observations of the COSMOS field. Search for X-ray clusters of galaxies.
in source:	NAME COSMOS Field
Ref:	=2007ApJS..172..182F
by	FINOGUENOV A. , GUZZO L., HASINGER G., SCOVILLE N.Z., AUSSEL H., BOHRINGER H., BRUSA M., CAPAK P., CAPPELLUTI N., COMASTRI A., GIODINI S., GRIFFITHS R.E., IMPEY C., KOEKEMOER A.M., KNEIB J.-P., LEAUTHAUD A., LE FEVRE O., LILLY S., MAINIERI V., MASSEY R., McCRACKEN H.J., MOBASHER B., MURAYAMA T., PEACOCK J.A., SAKELLIOU I., SCHINNERER E., SILVERMAN J.D., SMOLCIC V., TANIGUCHI Y., TASCA L., TAYLOR J.E., TRUMP J.R., ZAMORANI G.
	Astrophys. J., Suppl. Ser., 172, 182-195 (2007)
	The XMM-Newton wide-field survey in the COSMOS field: statistical properties of clusters of galaxies.
o	Table 1: <[FGH2007] NNN> N=72 among (Nos 3-145).
=E=	Catalogue in electronic form as J/ApJS/172/182
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FGH2019]
[FGH2019]	(Fahrion+Georgiev+Hilker+, 2019)
Write:	<<[FGH2019] FCC 47-UCD1>>
N:	1
Object:	UCD (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT MUSE observations of N=1 ultra compact dwarf in the field of FCC 47. Use of HST ACS archival data.
Ref:	=2019A&A...625A..50F
by	FAHRION K. , GEORGIEV I., HILKER M., LYUBENOVA M., VAN DE VEN G., ALFARO-CUELLO M., CORSINI E.M., SARZI M., McDERMID R.M., DE ZEEUW T.
	Astron. Astrophys., 625A, 50-50 (2019)
	Single metal-poor ultra compact dwarf galaxy at one kiloparsec distance from the low-mass elliptical galaxy FCC 47.
o	<[FGH2019] FCC 47-UCD1> N=1.
=E=	Catalogue in electronic form as <J/A+A/625/A50/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FGK2003]
[FGK2003]	(Figer+Gilmore+Kim+, 2003)
Write:	<<[FGK2003] NNN>>
N:	85
Object:	Cool * (SIMBAD class: Star)
Note:	Radial velocities of 85 cool stars projected onto the central parsec of the galaxy. See also [GPE2000].
in source:	NAME Gal Center
Ref:	=2003ApJ...599.1139F
by	FIGER D.F. , GILMORE D., KIM S.S., MORRIS M., BECKLIN E.E., McLEAN I.S., GILBERT A.M., GRAHAM J.R., LARKIN J.E., LEVENSON N.A., TEPLITZ H.I.
	Astrophys. J., 599, 1139-1156 (2003)
	High-precision stellar radial velocities in the Galactic Center.
o	(Erratum) erratum vol. 611, p. 1209 (2004)
o	Table 3: * kap Tau not identified. Table 4: format GNNNNA = [GPE2000] NN.NNA in SIMBAD.
o	Table 4: <[FGK2003] NNN> N=85 among (Nos 68-580).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 0FGL
0FGL	(Fermi/LAT Bright Gamma-Ray Source, preliminary list)
Write:	<<0FGL JHHMM.m+DDMM>>
N:	205
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	FERMI/LAT (Large Area Telescope) bright gamma-ray source list. The 0 prefix refers to the preliminary nature of the list. 2009ApJ...695L..72A: First reference with 0FGL objects.
Ref:	=2009ApJ...695L..72A
by	ABDO A.A. , ACKERMANN M., ATWOOD W.B., BALDINI L., BALLET J., BARBIELLINI G., BARING M.G., BASTIERI D., BAUGHMAN B.M., BECHTOL K., BELLAZZINI R., BERENJI B., BLOOM E.D., BONAMENTE E., BORGLAND A.W., BREGEON J., BREZ A., BRIGIDA M., BRUEL P., BURNETT T.H., CALIANDRO G.A., CAMERON R.A., CARAVEO P.A., CASANDJIAN J.M., CECCHI C., CHARLES E., CHEKHTMAN A., CHEUNG C.C., CHIANG J., CIPRINI S., CLAUS R., COHEN-TANUGI J., COMINSKY L.R., CONRAD J., DERMER C.D., DE ANGELIS A., DE PALMA F., DIGEL S.W., DONATO D., DORMODY M., DO COUTO E SILVA E., DRELL P.S., DUBOIS R., DUMORA D., EDMONDS Y., FARNIER C., FAVUZZI C., FLEURY P., FOCKE W.B., FRAILIS M., FUKAZAWA Y., FUNK S., FUSCO P., GARGANO F., GASPARRINI D., GEHRELS N., GERMANI S., GIEBELS B., GIGLIETTO N., GIORDANO F., GLANZMAN T., GODFREY G., GRENIER I.A., GRONDIN M.-H., GROVE J.E., GUILLEMOT L., GUIRIEC S., HARDING A.K., HAYASHIDA M., HAYS E., HUGHES R.E., JOHANNESSON G., JOHNSON A.S., JOHNSON R.P., JOHNSON T.J., JOHNSON W.N., JOHNSTON S., KAMAE T., KATAGIRI H., KATAOKA J., KAWAI N., KERR M., KNODLSEDER J., KOMIN N., KRAMER M., KUEHN F., KUSS M., LATRONICO L., LEE S.-H., LEMOINE-GOUMARD M., LONGO F., LOPARCO F., LOTT B., LOVELLETTE M.N., LUBRANO P., MAKEEV A., MARELLI M., MAZZIOTTA M.N., McCONVILLE W., McENERY J.E., MEURER C., MICHELSON P.F., MITTHUMSIRI W., MIZUNO T., MOISEEV A.A., MONTE C., MONZANI M.E., MORSELLI A., MOSKALENKO I.V., MURGIA S., NOLAN P.L., NUSS E., OHSUGI T., OMODEI N., ORLANDO E., ORMES J.F., PANEQUE D., PANETTA J.H., PARENT D., PEPE M., PESCE-ROLLINS M., PIRON F., PORTER T.A., RAINO S., RANDO R., RAZZANO M., REIMER A., REIMER O., REPOSEUR T., RITZ S., ROCHESTER L.S., RODRIGUEZ A.Y., ROMANI R.W., ROTH M., RYDE F., SADROZINSKI H.F.-W., SANCHEZ D., SANDER A., SAZ PARKINSON P.M., SGRO C., SISKIND E.J., SMITH D.A., SMITH P.D., SPANDRE G., SPINELLI P., STARCK J.-L., STRICKMAN M.S., SUSON D.J., TAJIMA H., TAKAHASHI H., TANAKA T., THAYER J.B., THAYER J.G., THOMPSON D.J., THORSETT S.E., TIBALDO L., TORRES D.F., TOSTI G., TRAMACERE A., UCHIYAMA Y., USHER T.L., VAN ETTEN A., VILCHEZ N., VITALE V., WAITE A.P., WATTERS K., WOOD K.S., YLINEN T., ZIEGLER M., HOBBS G., KEITH M., MANCHESTER R.N., WELTEVREDE P.
	Astrophys. J., 695L, 72-77 (2009)
	Discovery of pulsed γ-rays from the young radio pulsar PSR J1028-5819 with the Fermi large area telescope.
o	PSR J1028+5819 is a misprint for PSR J1028-5819.
o	Text: <0FGL JHHMM.m+DDMM> N=3.
Ref:	=2009ApJS..183...46A
by	ABDO A.A. , ACKERMANN M., AJELLO M., ATWOOD W.B., AXELSSON M., BALDINI L., BALLET J., BAND D.L., BARBIELLINI G., BASTIERI D., BATTELINO M., BAUGHMAN B.M., BECHTOL K., BELLAZZINI R., BERENJI B., BIGNAMI G.F., BLANDFORD R.D., BLOOM E.D., BONAMENTE E., BORGLAND A.W., BOUVIER A., BREGEON J., BREZ A., BRIGIDA M., BRUEL P., BURNETT T.H., CALIANDRO G.A., CAMERON R.A., CARAVEO P.A., CASANDJIAN J.M., CAVAZZUTI E., CECCHI C., CHARLES E., CHEKHTMAN A., CHEUNG C.C., CHIANG J., CIPRINI S., CLAUS R., COHEN-TANUGI J., COMINSKY L.R., CONRAD J., CORBET R., COSTAMANTE L., CUTINI S., DAVIS D.S., DERMER C.D., DE ANGELIS A., DE LUCA A., DE PALMA F., DIGEL S.W., DORMODY M., DO COUTO E SILVA E., DRELL P.S., DUBOIS R., DUMORA D., FARNIER C., FAVUZZI C., FEGAN S.J., FERRARA E.C., FOCKE W.B., FRAILIS M., FUKAZAWA Y., FUNK S., FUSCO P., GARGANO F., GASPARRINI D., GEHRELS N., GERMANI S., GIEBELS B., GIGLIETTO N., GIOMMI P., GIORDANO F., GLANZMAN T., GODFREY G., GRENIER I.A., GRONDIN M.-H., GROVE J.E., GUILLEMOT L., GUIRIEC S., HANABATA Y., HARDING A.K., HARTMAN R.C., HAYASHIDA M., HAYS E., HEALEY S.E., HORAN D., HUGHES R.E., JOHANNESSON G., JOHNSON A.S., JOHNSON R.P., JOHNSON T.J., JOHNSON W.N., KAMAE T., KATAGIRI H., KATAOKA J., KAWAI N., KERR M., KNODLSEDER J., KOCEVSKI D., KOCIAN M.L., KOMIN N., KUEHN F., KUSS M., LANDE J., LATRONICO L., LEE S.-H., LEMOINE-GOUMARD M., LONGO F., LOPARCO F., LOTT B., LOVELLETTE M.N., LUBRANO P., MADEJSKI G.M., MAKEEV A., MARELLI M., MAZZIOTTA M.N., McCONVILLE W., McENERY J.E., McGLYNN S., MEURER C., MICHELSON P.F., MITTHUMSIRI W., MIZUNO T., MOISEEV A.A., MONTE C., MONZANI M.E., MORETTI E., MORSELLI A., MOSKALENKO I.V., MURGIA S., NAKAMORI T., NOLAN P.L., NORRIS J.P., NUSS E., OHNO M., OHSUGI T., OMODEI N., ORLANDO E., ORMES J.F., OZAKI M., PANEQUE D., PANETTA J.H., PARENT D., PELASSA V., PEPE M., PESCE-ROLLINS M., PIRON F., PORTER T.A., POUPARD L., RAINO S., RANDO R., RAY P.S., RAZZANO M., REA N., REIMER A., REIMER O., REPOSEUR T., RITZ S., ROCHESTER L.S., RODRIGUEZ A.Y., ROMANI R.W., ROTH M., RYDE F., SADROZINSKI H.F.-W., SANCHEZ D., SANDER A., SAZ PARKINSON P.M., SCARGLE J.D., SCHALK T.L., SELLERHOLM A., SGRO C., SHAW M.S., SHRADER C., SIERPOWSKA-BARTOSIK A., SISKIND E.J., SMITH D.A., SMITH P.D., SPANDRE G., SPINELLI P., STARCK J.-L., STEPHENS T.E., STRICKMAN M.S., STRONG A.W., SUSON D.J., TAJIMA H., TAKAHASHI H., TAKAHASHI T., TANAKA T., THAYER J.B., THAYER J.G., THOMPSON D.J., TIBALDO L., TIBOLLA O., TORRES D.F., TOSTI G., TRAMACERE A., UCHIYAMA Y., USHER T.L., VAN ETTEN A., VILCHEZ N., VITALE V., WAITE A.P., WALLACE E., WANG P., WATTERS K., WINER B.L., WOOD K.S., YLINEN T., ZIEGLER M., (The Fermi-LAT Collaboration)
	Astrophys. J., Suppl. Ser., 183, 46-66 (2009)
	Fermi/Large Area Telescope bright γ-ray source list.
o	Table 5: <0FGL JHHMM.m+DDMM> N=205.
=E=	Catalogue in electronic form as J/ApJS/183/46
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 1FGL
1FGL	(First Fermi/LAT catalog)
Write:	<<1FGL JHHMM.m+DDMM>> <<1FGL JHHMM.m+DDMMc>>
N:	1451
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Fermi is a NASA satellite launched in June 2008. The LAT instrument covers the range 30MeV to 300GeV. It provides a gamma-ray all-sky survey. The first Fermi catalog is provided by the LAT collaboration, based on data acquired between August 2008 and June 2009. More information can be found at http://fermi.gsfc.nasa.gov/ssc/ Publications by the LAT collaboration can be found at https://www-glast.stanford.edu/cgi-bin/pubpub/
Ref:	=2010ApJS..188..405A
by	ABDO A.A. , ACKERMANN M., AJELLO M., ALLAFORT A., ANTOLINI E., ATWOOD W.B., AXELSSON M., BALDINI L., BALLET J., BARBIELLINI G., BASTIERI D., BAUGHMAN B.M., BECHTOL K., BELLAZZINI R., BELLI F., BERENJI B., BISELLO D., BLANDFORD R.D., BLOOM E.D., BONAMENTE E., BONNELL J., BORGLAND A.W., BOUVIER A., BREGEON J., BREZ A., BRIGIDA M., BRUEL P., BURNETT T.H., BUSETTO G., BUSON S., CALIANDRO G.A., CAMERON R.A., CAMPANA R., CANADAS B., CARAVEO P.A., CARRIGAN S., CASANDJIAN J.M., CAVAZZUTI E., CECCANTI M., CECCHI C., CELIK O., CHARLES E., CHEKHTMAN A., CHEUNG C.C., CHIANG J., CILLIS A.N., CIPRINI S., CLAUS R., COHEN-TANUGI J., CONRAD J., CORBET R., DAVIS D.S., DEKLOTZ M., DEN HARTOG P.R., DERMER C.D., DE ANGELIS A., DE LUCA A., DE PALMA F., DIGEL S.W., DORMODY M., DO COUTO E SILVA E., DRELL P.S., DUBOIS R., DUMORA D., FABIANI D., FARNIER C., FAVUZZI C., FEGAN S.J., FERRARA E.C., FOCKE W.B., FORTIN P., FRAILIS M., FUKAZAWA Y., FUNK S., FUSCO P., GARGANO F., GASPARRINI D., GEHRELS N., GERMANI S., GIAVITTO G., GIEBELS B., GIGLIETTO N., GIOMMI P., GIORDANO F., GIROLETTI M., GLANZMAN T., GODFREY G., GRENIER I.A., GRONDIN M.-H., GROVE J.E., GUILLEMOT L., GUIRIEC S., GUSTAFSSON M., HADASCH D., HANABATA Y., HARDING A.K., HAYASHIDA M., HAYS E., HEALEY S.E., HILL A.B., HORAN D., HUGHES R.E., IAFRATE G., JOHANNESSON G., JOHNSON A.S., JOHNSON R.P., JOHNSON T.J., JOHNSON W.N., KAMAE T., KATAGIRI H., KATAOKA J., KAWAI N., KERR M., KNODLSEDER J., KOCEVSKI D., KUSS M., LANDE J., LANDRIU D., LATRONICO L., LEE S.-H., LEMOINE-GOUMARD M., LIONETTO A.M., LLENA GARDE M., LONGO F., LOPARCO F., LOTT B., LOVELLETTE M.N., LUBRANO P., MADEJSKI G.M., MAKEEV A., MARANGELLI B., MARELLI M., MASSARO E., MAZZIOTTA M.N., McCONVILLE W., McENERY J.E., MICHELSON P.F., MINUTI M., MITTHUMSIRI W., MIZUNO T., MOISEEV A.A., MONGELLI M., MONTE C., MONZANI M.E., MORETTI E., MORSELLI A., MOSKALENKO I.V., MURGIA S., NAKAJIMA H., NAKAMORI T., NAUMANN-GODO M., NOLAN P.L., NORRIS J.P., NUSS E., OHNO M., OHSUGI T., OMODEI N., ORLANDO E., ORMES J.F., OZAKI M., PACCAGNELLA A., PANEQUE D., PANETTA J.H., PARENT D., PELASSA V., PEPE M., PESCE-ROLLINS M., PINCHERA M., PIRON F., PORTER T.A., POUPARD L., RAINO S., RANDO R., RAY P.S., RAZZANO M., RAZZAQUE S., REA N., REIMER A., REIMER O., REPOSEUR T., RIPKEN J., RITZ S., ROCHESTER L.S., RODRIGUEZ A.Y., ROMANI R.W., ROTH M., SADROZINSKI H.F.-W., SALVETTI D., SANCHEZ D., SANDER A., SAZ PARKINSON P.M., SCARGLE J.D., SCHALK T.L., SCOLIERI G., SGRO C., SHAW M.S., SISKIND E.J., SMITH D.A., SMITH P.D., SPANDRE G., SPINELLI P., STARCK J.-L., STEPHENS T.E., STRIANI E., STRICKMAN M.S., STRONG A.W., SUSON D.J., TAJIMA H., TAKAHASHI H., TAKAHASHI T., TANAKA T., THAYER J.B., THAYER J.G., THOMPSON D.J., TIBALDO L., TIBOLLA O., TINEBRA F., TORRES D.F., TOSTI G., TRAMACERE A., UCHIYAMA Y., USHER T.L., VAN ETTEN A., VASILEIOU V., VILCHEZ N., VITALE V., WAITE A.P., WALLACE E., WANG P., WATTERS K., WINER B.L., WOOD K.S., YANG Z., YLINEN T., ZIEGLER M.
	Astrophys. J., Suppl. Ser., 188, 405-436 (2010)
	Fermi Large Area Telescope First Source Catalog.
o	Tables 2-3: <1FGL JHHMM.m+DDMMc> N=1451. DSM/IRFU/SAp, CEA Saclay
=E=	Catalogue in electronic form as J/ApJS/188/405
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: 2FGL
2FGL	(Second Fermi/LAT catalog)
Write:	<<2FGL JHHMM.m+DDMM>> <<2FGL JHHMM.m+DDMM{c\|e}>>
N:	1873
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Fermi is a NASA satellite launched in June 2008. The LAT instrument covers the range 30 MeV to 300 GeV. It provides a gamma-ray all-sky survey. The second Fermi catalog is provided by the LAT collaboration, based on data acquired between August 2008 and July 2010. More information can be found at http://fermi.gsfc.nasa.gov/ssc/ <\p> A letter "c" at the end of the format indicates that the source is considered to be potentially confused with Galactic diffuse emission. A letter "e" at the end of the format indicates that the source was included as an extended source in the analysis.
Ref:	=2012ApJS..199...31N
by	NOLAN P.L. , ABDO A.A., ACKERMANN M., AJELLO M., ALLAFORT A., ANTOLINI E., ATWOOD W.B., AXELSSON M., BALDINI L., BALLET J., BARBIELLINI G., BASTIERI D., BECHTOL K., BELFIORE A., BELLAZZINI R., BERENJI B., BIGNAMI G.F., BLANDFORD R.D., BLOOM E.D., BONAMENTE E., BONNELL J., BORGLAND A.W., BOTTACINI E., BOUVIER A., BRANDT T.J., BREGEON J., BRIGIDA M., BRUEL P., BUEHLER R., BURNETT T.H., BUSON S., CALIANDRO G.A., CAMERON R.A., CAMPANA R., CANADAS B., CANNON A., CARAVEO P.A., CASANDJIAN J.M., CAVAZZUTI E., CECCANTI M., CECCHI C., CELIK O., CHARLES E., CHEKHTMAN A., CHEUNG C.C., CHIANG J., CHIPAUX R., CIPRINI S., CLAUS R., COHEN-TANUGI J., COMINSKY L.R., CONRAD J., CORBET R., CUTINI S., D'AMMANDO F., DAVIS D.S., DE ANGELIS A., DECESAR M.E., DEKLOTZ M., DE LUCA A., DEN HARTOG P.R., DE PALMA F., DERMER C.D., DIGEL S.W., DO COUTO E SILVA E., DRELL P.S., DRLICA-WAGNER A., DUBOIS R., DUMORA D., ENOTO T., ESCANDE L., FABIANI D., FALLETTI L., FAVUZZI C., FEGAN S.J., FERRARA E.C., FOCKE W.B., FORTIN P., FRAILIS M., FUKAZAWA Y., FUNK S., FUSCO P., GARGANO F., GASPARRINI D., GEHRELS N., GERMANI S., GIEBELS B., GIGLIETTO N., GIOMMI P., GIORDANO F., GIROLETTI M., GLANZMAN T., GODFREY G., GRENIER I.A., GRONDIN M.-H., GROVE J.E., GUILLEMOT L., GUIRIEC S., GUSTAFSSON M., HADASCH D., HANABATA Y., HARDING A.K., HAYASHIDA M., HAYS E., HILL A.B., HORAN D., HOU X., HUGHES R.E., IAFRATE G., ITOH R., JOHANNESSON G., JOHNSON R.P., JOHNSON T.E., JOHNSON A.S., JOHNSON T.J., KAMAE T., KATAGIRI H., KATAOKA J., KATSUTA J., KAWAI N., KERR M., KNODLSEDER J., KOCEVSKI D., KUSS M., LANDE J., LANDRIU D., LATRONICO L., LEMOINE-GOUMARD M., LIONETTO A.M., LLENA GARDE M., LONGO F., LOPARCO F., LOTT B., LOVELLETTE M.N., LUBRANO P., MADEJSKI G.M., MARELLI M., MASSARO E., MAZZIOTTA M.N., McCONVILLE W., McENERY J.E., MEHAULT J., MICHELSON P.F., MINUTI M., MITTHUMSIRI W., MIZUNO T., MOISEEV A.A., MONGELLI M., MONTE C., MONZANI M.E., MORSELLI A., MOSKALENKO I.V., MURGIA S., NAKAMORI T., NAUMANN-GODO M., NORRIS J.P., NUSS E., NYMARK T., OHNO M., OHSUGI T., OKUMURA A., OMODEI N., ORLANDO E., ORMES J.F., OZAKI M., PANEQUE D., PANETTA J.H., PARENT D., PERKINS J.S., PESCE-ROLLINS M., PIERBATTISTA M., PINCHERA M., PIRON F., PIVATO G., PORTER T.A., RACUSIN J.L., RAINO S., RANDO R., RAZZANO M., RAZZAQUE S., REIMER A., REIMER O., REPOSEUR T., RITZ S., ROCHESTER L.S., ROMANI R.W., ROTH M., ROUSSEAU R., RYDE F., SADROZINSKI H.F.-W., SALVETTI D., SANCHEZ D.A., SAZ PARKINSON P.M., SBARRA C., SCARGLE J.D., SCHALK T.L., SGRO C., SHAW M.S., SHRADER C., SISKIND E.J., SMITH D.A., SPANDRE G., SPINELLI P., STEPHENS T.E., STRICKMAN M.S., SUSON D.J., TAJIMA H., TAKAHASHI H., TAKAHASHI T., TANAKA T., THAYER J.G., THAYER J.B., THOMPSON D.J., TIBALDO L., TIBOLLA O., TINEBRA F., TINIVELLA M., TORRES D.F., TOSTI G., TROJA E., UCHIYAMA Y., VANDENBROUCKE J., VAN ETTEN A., VAN KLAVEREN B., VASILEIOU V., VIANELLO G., VITALE V., WAITE A.P., WALLACE E., WANG P., WERNER M., WINER B.L., WOOD D.L., WOOD K.S., WOOD M., YANG Z., ZIMMER S.
	Astrophys. J., Suppl. Ser., 199, 31 (2012)
	Fermi Large Area Telescope second source catalog.
o	Table 4: <2FGL JHHMM.m+DDMM>, <2FGL JHHMM.m+DDMMc>, <2FGL JHHMM.m+DDMMe>, N=1873. DSM/IRFU/SAp, CEA Saclay
=E=	Catalogue in electronic form as <J/ApJS/199/31/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [FGL2003]
[FGL2003]	(Fergusson+Goods Treasury Team+Lee+, 2003)
Write:	<<[FGL2003] JHHMMSS.ss+DDMMSS.s>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations. Host galaxies of SN 2003AJ, SN 2003 AK, SN 2003AL.
Ref:	=2003IAUC.8069....1F
by	FERGUSON H.C. , (The GOODS Treasury Team), LEE K.S., (The Hubble Higher-Z Supernova Team), LOTOSS, WEISZ D., LI W.
	IAU Circ., 8069, 1-None (2003)
	Supernovae 2003aj, 2003ak, 2003al, 2003am, and 2003an.
o	<[FGL2003] JHHMMSS.ss+DDMMSS.s> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FGL2006]
[FGL2006]	(Fassnacht+Gal+Lubin+, 2006)
Write:	<<[FGL2006] Na>>
N:	4+2
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Keck LRIS and ESI observations. Spectroscopic survey of CLASS 1608+656 field: four groups of galaxies along the line of sight to CLASS are discovered. Group 1 is at the redshift of the lensing galaxies [KF99] 1608+656 G1 and G2, the 3 other groups are in the foreground of the lens.
Ref:	=2006ApJ...642...30F
by	FASSNACHT C.D. , GAL R.R., LUBIN L.M., McKEAN J.P., SQUIRES G.K., READHEAD A.C.S.
	Astrophys. J., 642, 30-38 (2006)
	Mass along the line of sight to the gravitational lens B1608+656: galaxy groups and implications for H_{0}.
o	Table 1: <[FGL2006] Na> (Nos 1-4, 4a-4b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 3FGL
3FGL	(Third Fermi/LAT catalog)
Write:	<<3FGL JHHMM.m+DDMM>> <<3FGL JHHMM.m+DDMM{c\|e\|i\|s}>>
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Fermi is a NASA satellite launched in June 2008. The LAT instrument covers the range 30 MeV to 300 GeV. It provides a gamma-ray all-sky survey. The third Fermi catalog is based on the first 4 yr of science data. More information can be found at http://fermi.gsfc.nasa.gov/ssc/ Format JHHMM.m+DDMMc\|e\|i\|s: m is decimal minutes of RA; in the name RA and DE are truncated at 0.1 decimal minutes and 1', respectively; "c" indicates that based on the region of the sky the source is considered to be potentially confused with Galactic diffuse emission; "e" indicates a source that was modeled as spatially extended ; the two spectral components of the Crab PWN are designated "i" and "s". See also 0FGL, 1FGL, 2FGL.
Ref:	=2015ApJS..218...23A
by	ACERO F. , ACKERMANN M., AJELLO M., ALBERT A., ATWOOD W.B., AXELSSON M., BALDINI L., BALLET J., BARBIELLINI G., BASTIERI D., BELFIORE A., BELLAZZINI R., BISSALDI E., BLANDFORD R.D., BLOOM E.D., BOGART J.R., BONINO R., BOTTACINI E., BREGEON J., BRITTO R.J., BRUEL P., BUEHLER R., BURNETT T.H., BUSON S., CALIANDRO G.A., CAMERON R.A., CAPUTO R., CARAGIULO M., CARAVEO P.A., CASANDJIAN J.M., CAVAZZUTI E., CHARLES E., CHAVES R.C.G., CHEKHTMAN A., CHEUNG C.C., CHIANG J., CHIARO G., CIPRINI S., CLAUS R., COHEN-TANUGI J., COMINSKY L.R., CONRAD J., CUTINI S., D'AMMANDO F., DE ANGELIS A., DEKLOTZ M., DE PALMA F., DESIANTE R., DIGEL S.W., DI VENERE L., DRELL P.S., DUBOIS R., DUMORA D., FAVUZZI C., FEGAN S.J., FERRARA E.C., FINKE J., FRANCKOWIAK A., FUKAZAWA Y., FUNK S., FUSCO P., GARGANO F., GASPARRINI D., GIEBELS B., GIGLIETTO N., GIOMMI P., GIORDANO F., GIROLETTI M., GLANZMAN T., GODFREY G., GRENIER I.A., GRONDIN M.-H., GROVE J.E., GUILLEMOT L., GUIRIEC S., HADASCH D., HARDING A.K., HAYS E., HEWITT J.W., HILL A.B., HORAN D., IAFRATE G., JOGLER T., JOHANNESSON G., JOHNSON R.P., JOHNSON A.S., JOHNSON T.J., JOHNSON W.N., KAMAE T., KATAOKA J., KATSUTA J., KUSS M., LA MURA G., LANDRIU D., LARSSON S., LATRONICO L., LEMOINE-GOUMARD M., LI J., LI L., LONGO F., LOPARCO F., LOTT B., LOVELLETTE M.N., LUBRANO P., MADEJSKI G.M., MASSARO F., MAYER M., MAZZIOTTA M.N., McENERY J.E., MICHELSON P.F., MIRABAL N., MIZUNO T., MOISEEV A.A., MONGELLI M., MONZANI M.E., MORSELLI A., MOSKALENKO I.V., MURGIA S., NUSS E., OHNO M., OHSUGI T., OMODEI N., ORIENTI M., ORLANDO E., ORMES J.F., PANEQUE D., PANETTA J.H., PERKINS J.S., PESCE-ROLLINS M., PIRON F., PIVATO G., PORTER T.A., RACUSIN J.L., RANDO R., RAZZANO M., RAZZAQUE S., REIMER A., REIMER O., REPOSEUR T., ROCHESTER L.S., ROMANI R.W., SALVETTI D., SANCHEZ-CONDE M., SAZ PARKINSON P.M., SCHULZ A., SISKIND E.J., SMITH D.A., SPADA F., SPANDRE G., SPINELLI P., STEPHENS T.E., STRONG A.W., SUSON D.J., TAKAHASHI H., TAKAHASHI T., TANAKA Y., THAYER J.G., THAYER J.B., THOMPSON D.J., TIBALDO L., TIBOLLA O., TORRES D.F., TORRESI E., TOSTI G., TROJA E., VAN KLAVEREN B., VIANELLO G., WINER B.L., WOOD K.S., WOOD M., ZIMMER S.
	Astrophys. J., Suppl. Ser., 218, 23 (2015)
	Fermi Large Area Telescope third source catalog.
o	Table 4: <3FGL JHHMM.m+DDMM> N=2929, <3FGL JHHMM.m+DDMMc> N=78, <3FGL JHHMM.m+DDMMe> N=25, <3FGL J0534.5+2201i> N=1, <3FGL J0534.5+2201s> N=1.
=E=	Catalogue in electronic form as <J/ApJS/218/23/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 4FGL
4FGL	(Fourth Fermi/LAT catalog)
Write:	<<4FGL JHHMM.m+DDMM>> <<4FGL JHHMM.m+DDMM{c\|e\|i\|s}>>
N:	6659
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Fermi is a NASA satellite launched in June 2008. The LAT instrument covers the range 30 MeV to 300 GeV. It provides a gamma-ray all-sky survey. The third Fermi catalog is based on the first 4 yr of science data. More information can be found at http://fermi.gsfc.nasa.gov/ssc/ Format JHHMM.m+DDMMc\|e\|i\|s: m is decimal minutes of RA; in the name RA and DE are rounded; the letter at the end can be: "c" (coincident with interstellar clump), "e" (extended source), "i" (for Crab nebula inverse Compton), or "s" (for Crab nebula synchrotron). The LAT catalogs and associated products of the various data releases are available at https://fermi.gsfc.nasa.gov/ssc/data/access/ LAT 8-year Source Catalog (4FGL) : N=5065 sources LAT 10-year Source Catalog (4FGL-DR2) : N=5788 sources LAT 12-year Source Catalog (4FGL-DR3) : N=6658 sources See also 0FGL, 1FGL, 2FGL, 3FGL.
Ref:	=2020ApJS..247...33A
by	ABDOLLAHI S. , ACERO F., ACKERMANN M., AJELLO M., ATWOOD W.B., AXELSSON M., BALDINI L., BALLET J., BARBIELLINI G., BASTIERI D., BECERRA GONZALEZ J., BELLAZZINI R., BERRETTA A., BISSALDI E., BLANDFORD R.D., BLOOM E.D., BONINO R., BOTTACINI E., BRANDT T.J., BREGEON J., BRUEL P., BUEHLER R., BURNETT T.H., BUSON S., CAMERON R.A., CAPUTO R., CARAVEO P.A., CASANDJIAN J.M., CASTRO D., CAVAZZUTI E., CHARLES E., CHATY S., CHEN S., CHEUNG C.C., CHIARO G., CIPRINI S., COHEN-TANUGI J., COMINSKY L.R., CORONADO-BLAZQUEZ J., COSTANTIN D., CUOCO A., CUTINI S., D'AMMANDO F., DEKLOTZ M., DE LA TORRE LUQUE P., DE PALMA F., DESAI A., DIGEL S.W., DI LALLA N., DI MAURO M., DI VENERE L., DOMINGUEZ A., DUMORA D., FANA DIRIRSA F., FEGAN S.J., FERRARA E.C., FRANCKOWIAK A., FUKAZAWA Y., FUNK S., FUSCO P., GARGANO F., GASPARRINI D., GIGLIETTO N., GIOMMI P., GIORDANO F., GIROLETTI M., GLANZMAN T., GREEN D., GRENIER I.A., GRIFFIN S., GRONDIN M.-H., GROVE J.E., GUIRIEC S., HARDING A.K., HAYASHI K., HAYS E., HEWITT J.W., HORAN D., JOHANNESSON G., JOHNSON T.J., KAMAE T., KERR M., KOCEVSKI D., KOVAC'EVIC' M., KUSS M., LANDRIU D., LARSSON S., LATRONICO L., LEMOINE-GOUMARD M., LI J., LIODAKIS I., LONGO F., LOPARCO F., LOTT B., LOVELLETTE M.N., LUBRANO P., MADEJSKI G.M., MALDERA S., MALYSHEV D., MANFREDA A., MARCHESINI E.J., MARCOTULLI L., MARTI-DEVESA G., MARTIN P., MASSARO F., MAZZIOTTA M.N., McENERY J.E., MEREU I., MEYER M., MICHELSON P.F., MIRABAL N., MIZUNO T., MONZANI M.E., MORSELLI A., MOSKALENKO I.V., NEGRO M., NUSS E., OJHA R., OMODEI N., ORIENTI M., ORLANDO E., ORMES J.F., PALATIELLO M., PALIYA V.S., PANEQUE D., PEI Z., PENA-HERAZO H., PERKINS J.S., PERSIC M., PESCE-ROLLINS M., PETROSIAN V., PETROV L., PIRON F., POON H., PORTER T.A., PRINCIPE G., RAINO S., RANDO R., RAZZANO M., RAZZAQUE S., REIMER A., REIMER O., REMY Q., REPOSEUR T., ROMANI R.W., SAZ PARKINSON P.M., SCHINZEL F.K., SERINI D., SGRO C., SISKIND E.J., SMITH D.A., SPANDRE G., SPINELLI P., STRONG A.W., SUSON D.J., TAJIMA H., TAKAHASHI M.N., TAK D., THAYER J.B., THOMPSON D.J., TIBALDO L., TORRES D.F., TORRESI E., VALVERDE J., VAN KLAVEREN B., VAN ZYL P., WOOD K., YASSINE M., ZAHARIJAS G.
	Astrophys. J., Suppl. Ser., 247, 33-33 (2020)
	Fermi Large Area Telescope fourth source catalog.
o	<4FGL JHHMM.m+DDMM> N=4899, <4FGL JHHMM.m+DDMMc> N=90, <4FGL JHHMM.m+DDMMe> N=74, <4FGL J0534.5+2201i> N=1, <4FGL J0534.5+2201s> N=1.
Ref:	=arXiv:2005.11208
Ref:	=2022ApJS..260...53A
by	ABDOLLAHI S. , ACERO F., BALDINI L., BALLET J., BASTIERI D., BELLAZZINI R., BERENJI B., BERRETTA A., BISSALDI E., BLANDFORD R.D., BLOOM E., BONINO R., BRILL A., BRITTO R.J., BRUEL P., BURNETT T.H., BUSON S., CAMERON R.A., CAPUTO R., CARAVEO P.A., CASTRO D., CHATY S., CHEUNG C.C., CHIARO G., CIBRARIO N., CIPRINI S., CORONADO-BLAZQUEZ J., CRNOGORCEVIC M., CUTINI S., D'AMMANDO F., DE GAETANO S., DIGEL S.W., DI LALLA N., DIRIRSA F., DI VENERE L., DOMINGUEZ A., FALLAH RAMAZANI V., FEGAN S.J., FERRARA E.C., FIORI A., FLEISCHHACK H., FRANCKOWIAK A., FUKAZAWA Y., FUNK S., FUSCO P., GALANTI G., GAMMALDI V., GARGANO F., GARRAPPA S., GASPARRINI D., GIACCHINO F., GIGLIETTO N., GIORDANO F., GIROLETTI M., GLANZMAN T., GREEN D., GRENIER I.A., GRONDIN M.-H., GUILLEMOT L., GUIRIEC S., GUSTAFSSON M., HARDING A.K., HAYS E., HEWITT J.W., HORAN D., HOU X., JOHANNESSON G., KARWIN C., KAYANOKI T., KERR M., KUSS M., LANDRIU D., LARSSON S., LATRONICO L., LEMOINE-GOUMARD M., LI J., LIODAKIS I., LONGO F., LOPARCO F., LOTT B., LUBRANO P., MALDERA S., MALYSHEV D., MANFREDA A., MARTI-DEVESA G., MAZZIOTTA M.N., MEREU I., MEYER M., MICHELSON P.F., MIRABAL N., MITTHUMSIRI W., MIZUNO T., MOISEEV A.A., MONZANI M.E., MORSELLI A., MOSKALENKO I.V., NEGRO M., NUSS E., OMODEI N., ORIENTI M., ORLANDO E., PANEQUE D., PEI Z., PERKINS J.S., PERSIC M., PESCE-ROLLINS M., PETROSIAN V., PILLERA R., POON H., PORTER T.A., PRINCIPE G., RAINO S., RANDO R., RANI B., RAZZANO M., RAZZAQUE S., REIMER A., REIMER O., REPOSEUR T., SANCHEZ-CONDE M., SAZ PARKINSON P.M., SCOTTON L., SERINI D., SGRO C., SISKIND E.J., SMITH D.A., SPANDRE G., SPINELLI P., SUEOKA K., SUSON D.J., TAJIMA H., TAK D., THAYER J.B., THOMPSON D.J., TORRES D.F., TROJA E., VALVERDE J., WOOD K., ZAHARIJAS G.
	Astrophys. J., Suppl. Ser., 260, 53-53 (2022)
	Incremental Fermi Large Area Telescope Fourth Source Catalog.
o	<4FGL JHHMM.m+DDMM> N=6266, <4FGL JHHMM.m+DDMMc> N=314, <4FGL JHHMM.m+DDMMe> N=77, <4FGL J0534.5+2201i> N=1, <4FGL J0534.5+2201s> N=1.
=E=	Catalogue in electronic form as <J/ApJS/247/33/>
=E=	Catalogue in electronic form as <IX/67/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FGM2003]
[FGM2003]	(Favata+Giardino+Micela+, 2003)= (FGMSD03)
Write:	<<[FGM2003] NN>> <<[FGM2003] SNN>>
N:	81
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	N=81 XMM-Newton sources in the LDN 1551 region. The 27 brightest sources have also a format 'SNN'.
Ref:	=2003A&A...403..187F
by	FAVATA F. , GIARDINO G., MICELA G., SCIORTINO S., DAMIANI F.
	Astron. Astrophys., 403, 187-203 (2003)
	An XMM-Newton-based X-ray survey of pre-main sequence stellar emission in the L1551 star-forming complex.
o	Table 1: <[FGM2003] NN> (Nos 1-81). Table 2: <[FGM2003] SNN> (Nos S1-S27).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FGM2015]
[FGM2015]	(Fernandes+Gregorio-Hetem+Montmerle+, 2015)
Write:	<<[FGM2015] NNa>>
N:	83
Object:	* (SIMBAD class: Star)
Note:	Gemini South GMOS observations of N=83 stars associated with the Sh 2-296 nebula. Use of NOMAD, 2MASS, and WISE archival data.
in source:	SH 2-296
Ref:	=2015MNRAS.448..119F
by	FERNANDES B. , GREGORIO-HETEM J., MONTMERLE T., ROJAS G.
	Mon. Not. R. Astron. Soc., 448, 119-134 (2015)
	Spectroscopic characterization of X-ray emitting young stars associated with the Sh 2-296 nebula.
o	Tables 3-4: <[FGM2015] NNa> N=83 among (Nos 1-75).
o	In references, the bibcode for Rebull et al. 2013 is 2013AJ....145...15R (not ApJ).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FGM91]
[FGM91]	(Falomo+Giraud+Maraschi+, 1998)
Write:	<<[FGM91] GN>>
N:	6
Object:	G (SIMBAD class: Galaxy)
Note:	Galaxies around PKS 2155-304. Galaxy G1 is a companion galaxy to PKS 2155-304.
Ref:	=1991ApJ...380L..67F
by	FALOMO R. , GIRAUD E., MARASCHI L., MELNICK J., TANZI E.G., TREVES A.
	Astrophys. J., 380, 67-69 (1991)
	On the nebulosity surrounding the BL Lacertae object PKS 2155-304.
o	Fig.2: <[FGM91] GN> (Nos G1-G3).
Ref:	=1993ApJ...411L..63F
by	FALOMO R. , PESCE J.E., TREVES A.
	Astrophys. J., 411, 63-66 (1993)
	The environment of the BL Lacertae object PKS 2155-304.
o	Fig.1: <[FGM91] GN> (No. G4) added.
Ref:	=2013AJ....145...73L
by	LIUZZO E. , FALOMO R., TREVES A., ARCIDIACONO C., TORRESI E., USLENGHI M., FARINATO J., MORETTI A., RAGAZZONI R., DIOLAITI E., LOMBINI M., BRAST R., DONALDSON R., KOLB J., MARCHETTI E., TORDO S.
	Astron. J., 145, 73 (2013)
	On the radio and near-infrared jet of PKS 2155-304 and its close environment.
o	Star S (Fig.1) = USNO-B1.0 0597-0939577
o	Figs 1+3, Tables 1-2: <[FGM91] GN> (Nos G5-G6) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FGMSD03
FGMSD03	(Favata+Giardino+Micela+Sciotino+Damiani)
*****	Avoid the usage of FGMSD03, prefer [FGM2003]
Origin	of the Acronym: L (2007A&A...468..391G)
Details on Acronym: [FGR96]
[FGR96]	(Frail+Goss+Reynoso+, 1996)
Write:	<<[FGR96] HHMMSS.s+DDMMSS>> <<[FGR96] HHMMSS.s+DDMMSS.s>> <<[FGR96] HHMMSS.ss+DDMMSS>> <<[FGR96] HHMMSS.ss+DDMMSS.s>>
N:	21
Object:	OH Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	N=21 OH maser features in 5 SNR
Ref:	=1996AJ....111.1651F
by	FRAIL D.A. , GOSS W.M., REYNOSO E.M., GIACANI E.B., GREEN A.J., OTRUPCEK R.
	Astron. J., 111, 1651-1659 (1996)
	A survey for OH (1720 MHz) maser emission toward supernova remnants.
o	Table 2: <[FGR96] HHMMSS.s-DDMMSS>, <[FGR96] HHMMSS.s-DDMMSS.s>, <[FGR96] HHMMSS.ss-DDMMSS>, <[FGR96] HHMMSS.ss-DDMMSS.s>, N=21.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FGS
FGS	(Fine Guidance Sensor) (Not yet in Simbad)
Write:	<<FGS AA-NN>>
N:	99
Object:	* (SIMBAD class: Star)
Note:	Data from Fine Guidance Sensor interferometer on the HST. N=11 reference stars for each of the 9 Cepheids studied. In the format the letters AA stands for the name of the Ce* (ex. TV for T Vul).
Ref:	=2007AJ....133.1810B
by	BENEDICT G.F. , McARTHUR B.E., FEAST M.W., BARNES T.G., HARRISON T.E., PATTERSON R.J., MENZIES J.W., BEAN J.L., FREEDMAN W.L.
	Astron. J., 133, 1810-1827 (2007)
	Hubble Space Telescope fine guidance sensor parallaxes of galactic cepheid variable stars: period-luminosity relations.
o	(Erratum) erratum vol. 133, p. 2908 (2007)
o	Table 1: <FGS AA-NN> N=11x9.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FGS2011]
[FGS2011]	(Fumagalli+Gavazzi+Scaramella+, 2011) (Not yet in Simbad)
Write:	<<[FGS2011] AN>>
N:	12
Object:	Blob (SIMBAD class: EmObj = Emission Object)
Note:	GALEX and LBT LBC observations of N=12 Hα emitting blobs in VCC 1217. The clumpier "knots" are labelled K1-K8 east to west, and the more diffuse "filaments" F1-F4.
in source:	VCC 1217 = IC 3418
Ref:	=2011A&A...528A..46F
by	FUMAGALLI M. , GAVAZZI G., SCARAMELLA R., FRANZETTI P.
	Astron. Astrophys., 528A, 46-46 (2011)
	Constraining the ages of the fireballs in the wake of the dIrr galaxy VCC 1217/IC 3418.
o	Figs 1-2, Table 2: <[FGS2011] AN> (Nos K1-K8, F1-F4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FGT
FGT	(Fast Gaia Transient)
*****	Avoid the usage of FGT, prefer [WJH2018]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FGT2011]
[FGT2011]	(Feigelson+Getman+Townsley+, 2011)
Write:	<<[FGT2011] CCCP-Cl NN>> <<[FGT2011] CCCP-Gp NN>> <<[FGT2011] CCCP-Cl A>>
N:	20+4+31
Object:	Assoc. (SIMBAD class: Association = Association of Stars)
Note:	N=20 principal X-ray-selected clusters and N=31 small X-ray-selected groups of probable Carina members. N=4 large-scale regions (Region 'A' around and between Trumpler 14 and 15; Region 'B' within and south of the Trumpler 16 complex; Region 'C' over the Collinder 228 area; Region 'D' represents all other widely distributed stars in the full sample). Use of data from the Chandra Carina Complex Project data.
Ref:	=2011ApJS..194....9F
by	FEIGELSON E.D. , GETMAN K.V., TOWNSLEY L.K., BROOS P.S., POVICH M.S., GARMIRE G.P., KING R.R., MONTMERLE T., PREIBISCH T., SMITH N., STASSUN K.G., WANG J., WOLK S., ZINNECKER H.
	Astrophys. J., Suppl. Ser., 194, 9 (2011)
	X-ray star clusters in the Carina complex.
o	Figs 1-2, Table 1: <[FGT2011] CCCP-Cl NN> (Nos 1-20), <[FGT2011] CCCP-Cl A> (Nos A-D). Fig. 2, Table 2: <[FGT2011] CCCP-Gp NN> (Nos 1-31).
=E=	Catalogue in electronic form as J/ApJS/194/9
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FGW
FGW	(Fergusson+Gallagher+Wyse)
Write:	<<FGW NNNNA>>
N:	6+8+3
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	KPNO 4m telescope optical spectroscopy of N=17 HII regions in 3 galaxies.
in source:	NGC 628
in source:	NGC 1058
in source:	NGC 6946
Ref:	=1998AJ....116..673F
by	FERGUSON A.M.N. , GALLAGHER J.S., WYSE R.F.G.
	Astron. J., 116, 673-690 (1998)
	The extreme outer regions of disk galaxies. I. Chemical abundances of H II regions.
o	Figs 1-3, Table 2: <FGW 628A> (Nos A-F), <FGW 1058A> (Nos A-H), <FGW 6946A> (Nos A-C).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FGW2000]
[FGW2000]	(Ferguson+Gallagher+Wyse, 2000)
Write:	<<[FGW2000] N>>
N:	8
Object:	Em-line source (SIMBAD class: EmObj = Emission Object)
Stat:	is completely incorporated in Simbad
Note:	N=8 emission-line sources in the vicinity of And IV galaxy. Map in Fig.3.
Ref:	=2000AJ....120..821F
by	FERGUSON A.M.N. , GALLAGHER J.S., WYSE R.F.G.
	Astron. J., 120, 821-832 (2000)
	On the nature of Andromeda IV.
o	Table 1: <[FGW2000] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FGW2010]
[FGW2010]	(Farrell+Gosling+Webb+, 2010)
Write:	<<[FGW2010] N>>
N:	4
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=4 candidate NIR counterpars to 2XMM J174016.0-290337. Use of UKIDSS-GPS data.
Ref:	=2010A&A...523A..50F
by	FARRELL S.A. , GOSLING A.J., WEBB N.A., BARRET D., ROSEN S.R., SAKANO M., PANCRAZI B.
	Astron. Astrophys., 523A, 50-50 (2010)
	A new 626 s periodic X-ray source in the direction of the Galactic Center.
o	Fig. 9, Tables 3-4: <[FGW2010] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FH
FH	(Fosbury+Hawarden)
Write:	<<FH A>> <<FH N>>
N:	6+4
Object:	G + Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
in source:	NAME Cartwheel Galaxy
Ref:	=1977MNRAS.178..473F
by	FOSBURY R.A.E. , HAWARDEN T.G.
	Mon. Not. R. Astron. Soc., 178, 473-487 (1977)
	A 0035 'the cartwheel' a large southern ring galaxy.
o	Table 1: <FH A> (Nos A-F), <FH N> (Nos 1-4)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [FH2000]
[FH2000]	(Forbes+Hau, 2000) (Not yet in Simbad)
Write:	<<[FH2000] +SSS.s+SSS.s>>
N:	145
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	N=145 prtoglobular cluster candidates in Ks image of NGC 3597, beyond 20 arcsec galacocentric distance.
in source:	NGC 3597
Ref:	=2000MNRAS.312..703F
by	FORBES D.A. , HAU G.K.T.
	Mon. Not. R. Astron. Soc., 312, 703-711 (2000)
	Imaging of the merging galaxy NGC 3597 and its population of protoglobular clusters.
o	Table 4: <[FH2000] +SSS.s+SSS.s> N=145.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FHA2000]
[FHA2000]	(Fynbo+Holland+Andersen+, 2000) (Not yet in Simbad)
Write:	<<[FHA2000] sN>>
N:	6
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=6 objects in the field of SN 1998BW.
Ref:	=2000ApJ...542L..89F
by	FYNBO J.U. , HOLLAND S., ANDERSEN M.I., THOMSEN B., HJORTH J., BJORNSSON G., JAUNSEN A.O., NATARAJAN P., TANVIR N.
	Astrophys. J., 542, 89-93 (2000)
	Hubble space telescope space telescope imaging spectrograph imaging of the host galaxy of GRB 980425/SN 1998bw.
o	GRB 980919 is GRB 980910 (see 1999GCN...198....1K). (.)
o	Table 3: <[FHA2000] sN> (Nos s1-s6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FHB
FHB	(Field Horizontal-Branch)= ([Ph84])
Write:	<<FHB NN>>
N:	71
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Supersedes and continues 6 papers of Philip from 1967 to 1973, where Philip have given positions and finding charts for 60 Field Horizontal-Branch (FHB) stars
Ref:	=1984CoVVO...2....1P
by	PHILIP A.G.D.
	Contr. Van Vleck Obs., 2, 1-18 (1984)
	Finding charts for field horizontal-branch A-type stars.
o	cross-id. HLF not identified
o	<FHB NN> (Nos 1-71)
Origin	of the Acronym: L (1996AJ....112.2286C)
Details on Acronym: [FHB2012]
[FHB2012]	(Frye+Hurley+Bowen+, 2012)
Write:	<<[FHB2012] ELG NNNNN>> <<[FHB2012] ELS NNNNN>>
N:	52 (SIMBAD class: EmObj = Emission Object)
Note:	HST ACS grism observations of galaxies in the field of ACO 1689.
in source:	ACO 1689
Ref:	=2012ApJ...754...17F
by	FRYE B.L. , HURLEY M., BOWEN D.V., MEURER G., SHARON K., STRAUGHN A., COE D., BROADHURST T., GUHATHAKURTA P.
	Astrophys. J., 754, 17 (2012)
	Spatially resolved HST grism spectroscopy of a lensed emission line galaxy at z ~ 1.
o	Table 1, col(1): <[FHB2012] ELS NNNNN> N=51 among (Nos 486-20004). Table 2, col(1): <[FHB2012] ELG N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FHC96]
[FHC96]	(Ford+Hui+Ciardullo+, 1996)
Write:	<<[FHC96] FFNNN>> <<[FHC96] SFFNN>>
N:	294+21
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Table 3: N=294 PN in 7 fields in M 104. The fields are (Nos 10, 14, 15, 16, 17, 21, 22), and the format is 'FFNNN', where 'FF' stands for the field, and 'NNN' for a running number in each field. Table 4: N=21 Secondary reference stars in each field, format 'SFFNN' where S stands for 'Secondary Star'
in source:	M 104 = NGC 4594 = Sombrero Galaxy
Ref:	=1996ApJ...458..455F
by	FORD H.C. , HUI X., CIARDULLO R., JACOBY G.H., FREEMAN K.C.
	Astrophys. J., 458, 455-466 (1996)
	The stellar halo of M 104. I. A survey for planetary nebulae and the planetary nebula luminosity function distance.
o	Table 3: <[FHC96] FFNNN> N=294, Table 7: <[FHC96] SFFNN> N=21
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FHD2010]
[FHD2010]	(Fouque+Heyrovsky+Dong+, 2010)
Write:	<<[FHD2010] WW component>>
N:	2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	IRSF SIRIUS observations of the microlensing event OGLE 2008-BLG-290.
Ref:	=2010A&A...518A..51F
by	FOUQUE P. , HEYROVSKY D., DONG S., GOULD A., UDALSKI A., ALBROW M.D., BATISTA V., BEAULIEU J.-P., BENNETT D.P., BOND I.A., BRAMICH D.M., CALCHI NOVATI S., CASSAN A., COUTURES C., DIETERS S., DOMINIK M., DOMINIS PRESTER D., GREENHILL J., HORNE K., JORGENSEN U.G., KOZLOWSKI S., KUBAS D., LEE C.-H., MARQUETTE J.-B., MATHIASEN M., MENZIES J., MONARD L.A.G., NISHIYAMA S., PAPADAKIS I., STREET R., SUMI T., WILLIAMS A., YEE J.C., BRILLANT S., CALDWELL J.A.R., COLE A., COOK K.H., DONATOWICZ J., KAINS N., KANE S.R., MARTIN R., POLLARD K.R., SAHU K.C., TSAPRAS Y., WAMBSGANSS J., ZUB M., DEPOY D.L., GAUDI B.S., HAN C., LEE C.-U., PARK B.-G., POGGE R.W., KUBIAK M., SZYMANSKI M.K., PIETRZYNSKI G., SOSZYNSKI I., SZEWCZYK O., ULACZYK K., WYRZYKOWSKI L., ABE F., FUKUI A., FURUSAWA K., GILMORE A.C., HEARNSHAW J.B., ITOW Y., KAMIYA K., KILMARTIN P.M., KORPELA A.V., LIN W., LING C.H., MASUDA K., MATSUBARA Y., MIYAKE N., MURAKI Y., NAGAYA M., OHNISHI K., OKUMURA T., PERROTT Y., RATTENBURY N.J., SAITO T., SAKO T., SATO S., SKULJAN L., SULLIVAN D., SWEATMAN W., TRISTRAM P.J., YOCK P.C.M., ALLAN A., BODE M.F., BURGDORF M.J., CLAY N., FRASER S.N., HAWKINS E., KERINS E., LISTER T.A., MOTTRAM C.J., SAUNDERS E.S., SNODGRASS C., STEELE I.A., WHEATLEY P.J., ANGUITA T., BOZZA V., HARPSOE K., HINSE T.C., HUNDERTMARK M., KJAERGAARD P., LIEBIG C., MANCINI L., MASI G., RAHVAR S., RICCI D., SCARPETTA G., SOUTHWORTH J., SURDEJ J., THOENE C.C., RIFFESER A., SEITZ S., BENDER R.
	Astron. Astrophys., 518A, 51-51 (2010)
	OGLE 2008-BLG-290: an accurate measurement of the limb darkening of a galactic bulge K giant spatially resolved by microlensing.
o	Table 1: <[FHD2010] WW component> (Nos NE component, SW component).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FHD99]
[FHD99]	(Flores+Hammer+Desert+, 1999)= [FHT99] = (ISO)
Write:	<<[FHD99] ISO NNN>>
Object:	G + * + ? (SIMBAD class: Infrared = Infra-Red Source)
Note:	ISOCAM observations of a CFRS field 1415+52. See also [ELG99].
Ref:	=1999A&A...343..389F
by	FLORES H. , HAMMER F., DESERT F.X., CESARSKY C., THUAN T., CRAMPTON D., EALES S., LE FEVRE O., LILLY S.J., OMONT A., ELBAZ D.
	Astron. Astrophys., 343, 389-398 (1999)
	Deep Galaxy survey at 6.75µm with the ISO satellite.
o	Tables 1, 2: <[FHD99] ISO NNN> N=56 among (Nos 1-454).
Ref:	=1999ApJ...517..148F
by	FLORES H. , HAMMER F., THUAN T.X., CESARSKY C., DESERT F.X., OMONT A., LILLY S.J., EALES S., CRAMPTON D., LE FEVRE O.
	Astrophys. J., 517, 148-167 (1999)
	15 micron Infrared Space Observatory observations of the 1415+52 Canada-France redshift survey field: the cosmic star formation rate as derived from deep ultraviolet, optical, mid-infrared, and radio photometry.
o	Acronym [FHT99] is sometimes used for this ref., but it is the same acronym as [FHD99] (first ref. 1999A&A...343..389F)
o	Table 1: <[FHD99] ISO NNN> N=85 among (Nos 0-475).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FHES
FHES	(Fermi High-Latitude Extended Sources)
Write:	<<FHES JHHMM.m+DDMM>>
N:	95
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	N=95 extended sources, as part of the Fermi High-Latitude Extended Sources Catalog.
Ref:	=2018ApJS..237...32A
by	ACKERMANN M. , AJELLO M., BALDINI L., BALLET J., BARBIELLINI G., BASTIERI D., BELLAZZINI R., BISSALDI E., BLANDFORD R.D., BLOOM E.D., BONINO R., BOTTACINI E., BRANDT T.J., BREGEON J., BRUEL P., BUEHLER R., CAMERON R.A., CAPUTO R., CARAVEO P.A., CASTRO D., CAVAZZUTI E., CHARLES E., CHEUNG C.C., CHIARO G., CIPRINI S., COHEN-TANUGI J., COSTANTIN D., CUTINI S., D'AMMANDO F., DE PALMA F., DESAI A., DI LALLA N., DI MAURO M., DI VENERE L., FAVUZZI C., FINKE J., FRANCKOWIAK A., FUKAZAWA Y., FUNK S., FUSCO P., GARGANO F., GASPARRINI D., GIGLIETTO N., GIORDANO F., GIROLETTI M., GREEN D., GRENIER I.A., GUILLEMOT L., GUIRIEC S., HAYS E., HEWITT J.W., HORAN D., JOHANNESSON G., KENSEI S., KUSS M., LARSSON S., LATRONICO L., LEMOINE-GOUMARD M., LI J., LONGO F., LOPARCO F., LOVELLETTE M.N., LUBRANO P., MAGILL J.D., MALDERA S., MANFREDA A., MAZZIOTTA M.N., McENERY J.E., MEYER M., MIZUNO T., MONZANI M.E., MORSELLI A., MOSKALENKO I.V., NEGRO M., NUSS E., OMODEI N., ORIENTI M., ORLANDO E., ORMES J.F., PALATIELLO M., PALIYA V.S., PANEQUE D., PERKINS J.S., PERSIC M., PESCE-ROLLINS M., PIRON F., PORTER T.A., PRINCIPE G., RAINO S., RANDO R., RANI B., RAZZAQUE S., REIMER A., REIMER O., REPOSEUR T., SGRO C., SISKIND E.J., SPANDRE G., SPINELLI P., SUSON D.J., TAJIMA H., THAYER J.B., TIBALDO L., TORRES D.F., TOSTI G., VALVERDE J., VENTERS T.M., VOGEL M., WOOD K., WOOD M., ZAHARIJAS G., BITEAU J., (The Fermi-LAT Collaboration)
	Astrophys. J., Suppl. Ser., 237, 32-32 (2018)
	The search for spatial extension in high-latitude sources detected by the Fermi Large Area Telescope.
o	Tables 3-4: <FHES JHHMM.m+DDMM> N=95.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FHF2006]
[FHF2006]	(Ferrari+Hunstead+Feretti+, 2006)
Write:	<<[FHF2006] RNN>> <<[FHF2006] JHHMMSS+DDMMSS>>
N:	17
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA 13cm and 22cm observations of ACO 3921.
in source:	ACO 3921
Ref:	=2006A&A...457...21F
by	FERRARI C. , HUNSTEAD R.W., FERETTI L., MAUROGORDATO S., SCHINDLER S.
	Astron. Astrophys., 457, 21-34 (2006)
	ATCA observations of the galaxy cluster Abell 3921. I. Radio emission from the central merging sub-clusters.
o	Table 3: <[FHF2006] RNN> (Nos R1-R17) = <[FHF2006] JHHMMSS+DDMMSS> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FHH2003]
[FHH2003]	(Flynn+Holopainen+Holmberg, 2003)
Write:	<<[FHH2003] JHHMM+DDMMA>>
N:	1
Object:	WD (SIMBAD class: WhiteDwarf = White Dwarf)
Note:	J0050-5152A is the primary component of a binary. It's a White Dwarf. The secondary component is much fainter and its status as a WD is still to confirmed.
Ref:	=2003MNRAS.339..817F
by	FLYNN C. , HOLOPAINEN J., HOLMBERG J.
	Mon. Not. R. Astron. Soc., 339, 817-824 (2003)
	White dwarfs and Galactic dark matter.
o	Fig.1: <[FHH2003] J0050-5152A> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FHI77]
[FHI77]	(Felli+Habing+Israel, 1977)
Write:	<<[FHI77] S 252 ANNNN>>
N:	11+2
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Table 3: N=11 components of Sh 2-252A, Sh 2-252C, and Sh 2-252E, N=2 extended components observed at 1415MHz and 408MHz.
in source:	SH 2-252
Ref:	=1977A&A....59...43F
by	FELLI M. , HABING H.J., ISRAEL F.P.
	Astron. Astrophys., 59, 43-52 (1977)
	Aperture synthesis observations of galactic HII regions. V. The galactic nebula S252 (NGC 2175).
o	Table 3: <[FHI77] S 252 AN> (Nos A1-A3, C1-C4, E1-E4), <[FHI77] S 252 E1415>, <[FHI77] S 252 E408>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FHK
FHK	(Fang, Hillenbrand, Kim)
Write:	<<FHK NNN>>
N:	579
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	Palomar/Norris, WIYN/Hydra, Keck/DEIMOS, and MMT/Hectospec observations of NGC 7000 and IC 5070. List is Table 4 of Fang et al. 2021 https://iopscience.iop.org/article/10.3847/1538-4357/abba84#apjabba84t4
Notes:	We are planning to use these numbers in subsequent publications, so hope they can be designated as officially registered for Vizier.
Ref:	=2020ApJ...904..146F
by	FANG M. , HILLENBRAND L.A., KIM J.S., FINDEISEN K., HERCZEG G.J., CARPENTER J.M., REBULL L.M., WANG H.
	Astrophys. J., 904, 146-146 (2020)
	The first extensive spectroscopic study of young stars in the North America and Pelican Nebulae.
o	<FHK NNN> (Nos 1-580). California Institute of Technology
=E=	Catalogue in electronic form as <J/ApJ/904/146/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: 1FHL
1FHL	(First Fermi Hard LAT sources catalog)
Write:	<<1FHL JHHMM.m+DDMM>>
N:	514
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	Fermi is a NASA satellite launched in June 2008. The first Fermi catalog of hard sources is provided by the LAT collaboration. It is based on data from 10 to 500 GeV, acquired between August 2008 and July 2011. More information can be found at http://fermi.gsfc.nasa.gov/ssc/ See also 2FHL, 3FHL.
Ref:	=2013ApJS..209...34A
by	ACKERMANN M. , AJELLO M., ALLAFORT A., ATWOOD W.B., BALDINI L., BALLET J., BARBIELLINI G., BASTIERI D., BECHTOL K., BELFIORE A., BELLAZZINI R., BERNIERI E., BISSALDI E., BLOOM E.D., BONAMENTE E., BRANDT T.J., BREGEON J., BRIGIDA M., BRUEL P., BUEHLER R., BURNETT T.H., BUSON S., CALIANDRO G.A., CAMERON R.A., CAMPANA R., CARAVEO P.A., CASANDJIAN J.M., CAVAZZUTI E., CECCHI C., CHARLES E., CHAVES R.C.G., CHEKHTMAN A., CHEUNG C.C., CHIANG J., CHIARO G., CIPRINI S., CLAUS R., COHEN-TANUGI J., COMINSKY L.R., CONRAD J., CUTINI S., D'AMMANDO F., DE ANGELIS A., DE PALMA F., DERMER C.D., DESIANTE R., DIGEL S.W., DI VENERE L., DRELL P.S., DRLICA-WAGNER A., FAVUZZI C., FEGAN S.J., FERRARA E.C., FOCKE W.B., FORTIN P., FRANCKOWIAK A., FUNK S., FUSCO P., GARGANO F., GASPARRINI D., GEHRELS N., GERMANI S., GIGLIETTO N., GIOMMI P., GIORDANO F., GIROLETTI M., GODFREY G., GOMEZ-VARGAS G.A., GRENIER I.A., GUIRIEC S., HADASCH D., HANABATA Y., HARDING A.K., HAYASHIDA M., HAYS E., HEWITT J., HILL A.B., HORAN D., HUGHES R.E., JOGLER T., JOHANNESSON G., JOHNSON A.S., JOHNSON T.J., JOHNSON W.N., KAMAE T., KATAOKA J., KAWANO T., KNODLSEDER J., KUSS M., LANDE J., LARSSON S., LATRONICO L., LEMOINE-GOUMARD M., LONGO F., LOPARCO F., LOTT B., LOVELLETTE M.N., LUBRANO P., MASSARO E., MAYER M., MAZZIOTTA M.N., McENERY J.E., MEHAULT J., MICHELSON P.F., MIZUNO T., MOISEEV A.A., MONZANI M.E., MORSELLI A., MOSKALENKO I.V., MURGIA S., NEMMEN R., NUSS E., OHSUGI T., OKUMURA A., ORIENTI M., ORMES J.F., PANEQUE D., PERKINS J.S., PESCE-ROLLINS M., PIRON F., PIVATO G., PORTER T.A., RAINO S., RAZZANO M., REIMER A., REIMER O., REPOSEUR T., RITZ S., ROMANI R.W., ROTH M., SAZ PARKINSON P.M., SCHULZ A., SGRO C., SISKIND E.J., SMITH D.A., SPANDRE G., SPINELLI P., STAWARZ L., STRONG A.W., SUSON D.J., TAKAHASHI H., THAYER J.G., THAYER J.B., THOMPSON D.J., TIBALDO L., TINIVELLA M., TORRES D.F., TOSTI G., TROJA E., UCHIYAMA Y., USHER T.L., VANDENBROUCKE J., VASILEIOU V., VIANELLO G., VITALE V., WERNER M., WINER B.L., WOOD K.S., WOOD M.
	Astrophys. J., Suppl. Ser., 209, 34 (2013)
	The first Fermi-LAT catalog of sources above 10 GeV. DSM/IRFU/SAp, CEA Saclay
=E=	Catalogue in electronic form as J/ApJS/209/34
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: 2FHL
2FHL	(Second Fermi Hard LAT sources catalog)
Write:	<<2FHL JHHMM.m+DDMM>> <<2FHL JHHMM.m+DDMMe>>
N:	360
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	Catalog of N=360 hard sources detected in the 50GeV to 2TeV energy range, in 80 months of data. A letter "e" at the end of the format indicates an extended source. More information can be found at http://fermi.gsfc.nasa.gov/ssc/ See also 1FHL, 3FHL.
Ref:	=2016ApJS..222....5A
by	ACKERMANN M. , AJELLO M., ATWOOD W.B., BALDINI L., BALLET J., BARBIELLINI G., BASTIERI D., BECERRA GONZALEZ J., BELLAZZINI R., BISSALDI E., BLANDFORD R.D., BLOOM E.D., BONINO R., BOTTACINI E., BRANDT T.J., BREGEON J., BRUEL P., BUEHLER R., BUSON S., CALIANDRO G.A., CAMERON R.A., CAPUTO R., CARAGIULO M., CARAVEO P.A., CAVAZZUTI E., CECCHI C., CHARLES E., CHEKHTMAN A., CHEUNG C.C., CHIANG J., CHIARO G., CIPRINI S., COHEN J.M., COHEN-TANUGI J., COMINSKY L.R., CONRAD J., CUOCO A., CUTINI S., D'AMMANDO F., DE ANGELIS A., DE PALMA F., DESIANTE R., DI MAURO M., DI VENERE L., DOMINGUEZ A., DRELL P.S., FAVUZZI C., FEGAN S.J., FERRARA E.C., FOCKE W.B., FORTIN P., FRANCKOWIAK A., FUKAZAWA Y., FUNK S., FURNISS A.K., FUSCO P., GARGANO F., GASPARRINI D., GIGLIETTO N., GIOMMI P., GIORDANO F., GIROLETTI M., GLANZMAN T., GODFREY G., GRENIER I.A., GRONDIN M.-H., GUILLEMOT L., GUIRIEC S., HARDING A.K., HAYS E., HEWITT J.W., HILL A.B., HORAN D., IAFRATE G., HARTMANN D., JOGLER T., JOHANNESSON G., JOHNSON A.S., KAMAE T., KATAOKA J., KNODLSEDER J., KUSS M., LA MURA G., LARSSON S., LATRONICO L., LEMOINE-GOUMARD M., LI J., LI L., LONGO F., LOPARCO F., LOTT B., LOVELLETTE M.N., LUBRANO P., MADEJSKI G.M., MALDERA S., MANFREDA A., MAYER M., MAZZIOTTA M.N., MICHELSON P.F., MIRABAL N., MITTHUMSIRI W., MIZUNO T., MOISEEV A.A., MONZANI M.E., MORSELLI A., MOSKALENKO I.V., MURGIA S., NUSS E., OHSUGI T., OMODEI N., ORIENTI M., ORLANDO E., ORMES J.F., PANEQUE D., PERKINS J.S., PESCE-ROLLINS M., PETROSIAN V., PIRON F., PIVATO G., PORTER T.A., RAINO S., RANDO R., RAZZANO M., RAZZAQUE S., REIMER A., REIMER O., REPOSEUR T., ROMANI R.W., SANCHEZ-CONDE M., SAZ PARKINSON P.M., SCHMID J., SCHULZ A., SGRO C., SISKIND E.J., SPADA F., SPANDRE G., SPINELLI P., SUSON D.J., TAJIMA H., TAKAHASHI H., TAKAHASHI M., TAKAHASHI T., THAYER J.B., THOMPSON D.J., TIBALDO L., TORRES D.F., TOSTI G., TROJA E., VIANELLO G., WOOD K.S., WOOD M., YASSINE M., ZAHARIJAS G., ZIMMER S.
	Astrophys. J., Suppl. Ser., 222, 5 (2016)
	2FHL: the second catalog of hard Fermi-LAT sources.
o	Table 3: <2FHL JHHMM.m+DDMM> N=360. Tables 4-5: <2FHL JHHMM.m+DDMMe> N=20+5.
=E=	Catalogue in electronic form as <J/ApJS/222/5/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FHL2008]
[FHL2008]	(Fridriksson+Homan+Lewin+, 2008)
Write:	<<[FHL2008] NGC 6946 NN>> <<[FHL2008] NGC 4485-4490 NN>> <<[FHL2008] NGC 4485-4490 ULX-N>>
N:	90+38
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS observations of X-ray source variability in NGC 6946 and NGC 4485 + NGC 4490 pair.
in source:	NGC 6946
in source:	NGC 4485
in source:	NGC 4490
Ref:	=2008ApJS..177..465F
by	FRIDRIKSSON J.K. , HOMAN J., LEWIN W.H.G., KONG A.K.H., POOLEY D.
	Astrophys. J., Suppl. Ser., 177, 465-492 (2008)
	The long-term variability of the X-ray sources in NGC 6946 and NGC 4485/4490.
o	Table 2: <[FHL2008] NGC 6946 NN> (Nos 1-90). Table 6, col(1): <[FHL2008] NGC 4485-4490 NN> (Nos 1-38). Table 6, col(11): <[FHL2008] NGC 4485-4490 ULX-N> (Nos ULX-1 to ULX-8).
=E=	Catalogue in electronic form as J/ApJS/177/465
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 3FHL
3FHL	(Third Catalog of Hard Fermi-LAT Sources)
Write:	<<3FHL JHHMM.m+DDMM>> <<3FHL JHHMM.m+DDMMe>>
N:	1556
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	Catalog of N=1556 sources detected above 10GHz by the Fermi Large Area Telescope (LAT) in the first seven years of data. A letter "e" at the end of the format indicates an extended source. More information can be found at http://fermi.gsfc.nasa.gov/ssc/ See also 1FHL, 2FHL.
Ref:	=2017ApJS..232...18A
by	AJELLO M. , ATWOOD W.B., BALDINI L., BALLET J., BARBIELLINI G., BASTIERI D., BELLAZZINI R., BISSALDI E., BLANDFORD R.D., BLOOM E.D., BONINO R., BREGEON J., BRITTO R.J., BRUEL P., BUEHLER R., BUSON S., CAMERON R.A., CAPUTO R., CARAGIULO M., CARAVEO P.A., CAVAZZUTI E., CECCHI C., CHARLES E., CHEKHTMAN A., CHEUNG C.C., CHIARO G., CIPRINI S., COHEN J.M., COSTANTIN D., COSTANZA F., CUOCO A., CUTINI S., D'AMMANDO F., DE PALMA F., DESIANTE R., DIGEL S.W., DI LALLA N., DI MAURO M., DI VENERE L., DOMINGUEZ A., DRELL P.S., DUMORA D., FAVUZZI C., FEGAN S.J., FERRARA E.C., FORTIN P., FRANCKOWIAK A., FUKAZAWA Y., FUNK S., FUSCO P., GARGANO F., GASPARRINI D., GIGLIETTO N., GIOMMI P., GIORDANO F., GIROLETTI M., GLANZMAN T., GREEN D., GRENIER I.A., GRONDIN M.-H., GROVE J.E., GUILLEMOT L., GUIRIEC S., HARDING A.K., HAYS E., HEWITT J.W., HORAN D., JOHANNESSON G., KENSEI S., KUSS M., LA MURA G., LARSSON S., LATRONICO L., LEMOINE-GOUMARD M., LI J., LONGO F., LOPARCO F., LOTT B., LUBRANO P., MAGILL J.D., MALDERA S., MANFREDA A., MAZZIOTTA M.N., McENERY J.E., MEYER M., MICHELSON P.F., MIRABAL N., MITTHUMSIRI W., MIZUNO T., MOISEEV A.A., MONZANI M.E., MORSELLI A., MOSKALENKO I.V., NEGRO M., NUSS E., OHSUGI T., OMODEI N., ORIENTI M., ORLANDO E., PALATIELLO M., PALIYA V.S., PANEQUE D., PERKINS J.S., PERSIC M., PESCE-ROLLINS M., PIRON F., PORTER T.A., PRINCIPE G., RAINO S., RANDO R., RAZZANO M., RAZZAQUE S., REIMER A., REIMER O., REPOSEUR T., SAZ PARKINSON P.M., SGRO C., SIMONE D., SISKIND E.J., SPADA F., SPANDRE G., SPINELLI P., STAWARZ L., SUSON D.J., TAKAHASHI M., TAK D., THAYER J.G., THAYER J.B., THOMPSON D.J., TORRES D.F., TORRESI E., TROJA E., VIANELLO G., WOOD K., WOOD M.
	Astrophys. J., Suppl. Ser., 232, 18-18 (2017)
	3FHL: the Third Catalog of Hard Fermi-LAT Sources.
o	Table 3: <3FHL JHHMM.m+DDMM>, <3FHL JHHMM.m+DDMMe>, N=1556.
=E=	Catalogue in electronic form as <J/ApJS/232/18/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FHL98]
[FHL98]	(Feldt+Henning+Lagage+, 1998) (Not yet in Simbad)
Write:	<<[FHL98] A>>
N:	5
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
in source:	NAME Cha IRN
Ref:	=1998A&A...332..849F
by	FELDT M. , HENNING T., LAGAGE P.O., MANSKE V., SCHREYER K., STECKLUM B.
	Astron. Astrophys., 332, 849-856 (1998)
	The Chamaeleon infrared nebula revisited. Infrared imaging and spectroscopy of a young stellar object.
o	T.1: Sgr 9 = V* 9 Sgr?
o	Figs 1, 2, 3: <[FHL98] A> (Nos A-E)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FHM2006]
[FHM2006]	(Fesen+Hammell+Morse+, 2006)
Write:	<<[FHM2006] East N>>
N:	3
Object:	Knot (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	HST ACS and WFPC2 images of the SNE Cas A: 3 new ejecta knots are found in the eastern limb. See also [FG96] and [HF96] .
in source:	NAME Cas A
Ref:	=2006ApJ...636..859F
by	FESEN R.A. , HAMMELL M.C., MORSE J., CHEVALIER R.A., BORKOWSKI K.J., DOPITA M.A., GERARDY C.L., LAWRENCE S.S., RAYMOND J.C., VAN DEN BERGH S.
	Astrophys. J., 636, 859-872 (2006)
	Discovery of outlying high-velocity oxygen-rich ejecta in Cassiopeia A.
o	Table 3: <[FHM2006] East N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FHM2008]
[FHM2008]	(Furesz+Hartmann+Megeath+, 2008)
Write:	<<[FHM2008] FNN-apNNN>> <<[FHM2008] SN-apNNN>>
N:	1215
Object:	* in Cl* + * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	MMT 6.6m telescope spectroscopic observations of the ONC.
in source:	NAME ONC
Ref:	=2008ApJ...676.1109F
by	FURESZ G. , HARTMANN L.W., MEGEATH S.T., SZENTGYORGYI A.H., HAMDEN E.T.
	Astrophys. J., 676, 1109-1122 (2008)
	Kinematic structure of the Orion Nebula Cluster and its surroundings.
o	Tables 2-3, Col(2): <[FHM2008] FNN-apNNN>, <[FHM2008] SN-apNNN>, N=1215.
=E=	Catalogue in electronic form as <J/ApJ/676/1109/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FHM2009]
[FHM2009]	(Feron+Hjorth+McKean+, 2009) (Not yet in Simbad)
Write:	<<[FHM2009] SDSS JHHMM+DDMM>> <<[FHM2009] SDSS JHHMM+DDMM lens>> <<[FHM2009] SDSS JHHMM+DDMM source>> <<[FHM2009] Galaxy A>>
N:	8+8+8+5
Object:	Grav. lens + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	NOT observations of N=8 gravitational lens candidates. Use of SDSS data.
Ref:	=2009ApJ...696.1319F
by	FERON C. , HJORTH J., McKEAN J.P., SAMSING J.
	Astrophys. J., 696, 1319-1338 (2009)
	A search for disk-galaxy lenses in the Sloan Digital Sky Survey.
o	In Abstract, SDSS J081230.30+543650.9 is a misprint for SDSS J081213.30+543650.9.
o	Table 2: <[FHM2009] SDSS JHHMM+DDMM> N=8, <[FHM2009] SDSS JHHMM+DDMM lens> N=8, <[FHM2009] SDSS JHHMM+DDMM source> N=8. Table 6, Fig. 14: <[FHM2009] Galaxy A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FHM94]
[FHM94]	(Freedman+Hughes+Madore+, 1994)
Write:	<<[FHM94] CNN>> <<[FHM94] E1>>
N:	31+1
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Note:	HST WFPC observations. Tables 2, 3: (Nos C1-C31), letter 'C' in the format stands for 'Cepheid'. Table 6: No. E1, stands for Eclipsing variable. See also: [HST94], [KIF96], [FFH96], [SHM96], [GPF97], [RMM97], [PSF98], [FBK98], [HHH98], [TFS98], [GHS99], [KIS99], [SHF99], [GFF99], [MHS99], [SFK99], [PKB99], [GSF2000], [MHS2000]
in source:	M 81 = NGC 3031
Ref:	=1994ApJ...427..628F
by	FREEDMAN W.L. , HUGHES S.M., MADORE B.F., MOULD J.R., LEE M.G., STETSON P., KENNICUTT R.C., TURNER A., FERRARESE L., FORD H., GRAHAM J.A., HILL R., HOESSEL J.G., HUCHRA J., ILLINGWORTH G.D.
	Astrophys. J., 427, 628-655 (1994)
	The Hubble Space Telescope extragalactic distance scale key project. I. The discovery of cepheids and a new distance to M 81.
o	Tables 2, 3: <[FHM94] CNN> (Nos C1-C31). Table 6: <[FHM94] E1> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FHN2005]
[FHN2005]	(Freire+Hessels+Nice+, 2005)
Write:	<<[FHN2005] NGC 6760 Psr A>>
N:	2
Object:	ms Psr (SIMBAD class: Pulsar)
Stat:	is completely incorporated in Simbad
Note:	Arecibo and Green Bank observations of NGC 6760: N=2 millisecond pulsars, pulsar A was already known as PSR 1908+00.
in source:	NGC 6760
Ref:	=2005ApJ...621..959F
by	FREIRE P.C.C. , HESSELS J.W.T., NICE D.J., RANSOM S.M., LORIMER D.R., STAIRS I.H.
	Astrophys. J., 621, 959-965 (2005)
	The millisecond pulsars in NGC 6760.
o	<[FHN2005] NGC 6760 Psr A> (Nos A, B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FHO
FHO	(Findeisen+Hillenbrand+Ofek+, 2013)
Write:	<<FHO NN>>
N:	30
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	A Palomar Transient Factory (PTF) survey of N=30 sources in the North America complex.
in source:	NGC 7000 = NAME North America Nebula
Ref:	=2013ApJ...768...93F
by	FINDEISEN K. , HILLENBRAND L., OFEK E., LEVITAN D., SESAR B., LAHER R., SURACE J.
	Astrophys. J., 768, 93 (2013)
	Disk-related bursts and fades in young stars.
o	Tables 3-4: <FHO NN> (Nos 1-30).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FHP2006]
[FHP2006]	(Flores+Hammer+Puech+, 2006)= (HDFS)
Write:	<<[FHP2006] HDFS NNNN>>
N:	13 among N>5190
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spectroscopy with FLAMES-GIRAFFE at VLT of galaxies from HST images.
Ref:	=2006A&A...455..107F
by	FLORES H. , HAMMER F., PUECH M., AMRAM P., BALKOWSKI C.
	Astron. Astrophys., 455, 107-118 (2006)
	3D spectroscopy with VLT/GIRAFFE. I. The true Tully Fisher relationship at z ~ 0.6.
o	Table 2: Objects CFRS NNNNNN = CFRS HH.NNNN in SIMBAD.
o	Table 2, text: <[FHP2006] HDFS NNNN> N=13 among (Nos 4010-5190).
=E=	Catalogue in electronic form as J/A+A/455/107
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FHP2016]
[FHP2016]	(Fu+Hennawi+Prochaska+, 2016)
Write:	<<[FHP2016] DDD.dddd+DD.dddd>>
N:	13
Object:	smm G (SIMBAD class: Galaxy)
Note:	VLA 6 GHz radio continuum observations of N=13 Herschel submillimeter galaxies (SMGs). Additional LBT LUCI-1 NIR spectroscopic observations. Use of archival Herschel data.
Ref:	=2016ApJ...832...52F
by	FU H. , HENNAWI J.F., PROCHASKA J.X., MUTEL R., CASEY C., COORAY A., KERES D., ZHANG Z.-Y., CLEMENTS D., ISBELL J., LANG C., McGINNIS D., MICHALOWSKI M.J., MOOLEY K., PERLEY D., STOCKTON A., THOMPSON D.
	Astrophys. J., 832, 52-52 (2016)
	The circumgalactic medium of submillimeter galaxies. I. First results from a radio-identified sample.
o	Table 1: <[FHP2016] DDD.dddd+DD.dddd> N=13. Table 2: <[FHP2016] SMG JHHMMSS.ss+DDMMSS.s> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FHR82]
[FHR82]	(Fahlman+Hickson+Richer+, 1982)
Write:	<<[FHR82] A>> <<[FHR82] A'>> <<[FHR82] RN>> <<[FHR82] ggg>>
N:	19+2+2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	HRI observations of the Einstein Observatory. Stars in the field of 1E 2259+58.6: (Nos A-N, T, U, W, X)are candidates opt. counterpart, (No. B') is a companion to star B, (Nos R1-R2) are reference stars, (Nos gam, del) are 2 stars added in 1992. Maps.
Ref:	=1982ApJ...261L...1F
by	FAHLMAN G.G. , HICKSON P., RICHER H.B., GREGORY P.C., MIDDLEDITCH J.
	Astrophys. J., 261, 1-5 (1982)
	A possible optical counterpart to the X-ray pulsar 1E 2259+586.
o	Table 1: <[FHR82] A> (Nos A-B), <[FHR82] RN> (Nos R1-R2).
Ref:	=1983ApJ...274..313M
by	MIDDLEDITCH J. , PENNYPACKER C.R., BURNS M.S.
	Astrophys. J., 274, 313-326 (1983)
	Infrared and optical pulsations from HZ Herculis and possible 3.5 second infrared pulsations from 1E 2259+586.
o	Table 2: <[FHR82] A> (Nos C-D) added.
Ref:	=1991MNRAS.249..313D
by	DAVIES S.R. , COE M.J.
	Mon. Not. R. Astron. Soc., 249, 313-318 (1991)
	Optical and IR imaging of the locality of 1E 2259+586.
o	Tables 3, 4: <[FHR82] A> (Nos E-N) added, <[FHR82] B') N=1.
Ref:	=1992MNRAS.259..191C
by	COE M.J. , JONES L.R.
	Mon. Not. R. Astron. Soc., 259, 191-202 (1992)
	The continuing search for the optical counterpart of the enigmatic X-ray pulsar 1E 2259+586.
o	Fig.4: <[FHR82] A> (Nos T, U,) added, <[FHR82] aaa> (Nos gam, del).
Ref:	=1994MNRAS.270..178C
by	COE M.J. , JONES L.R., LEHTO H.
	Mon. Not. R. Astron. Soc., 270, 178-182 (1994)
	A deep radio search for the counterpart to the enigmatic X-ray pulsar 1E 2259+586.
o	Fig.2: <[FHR82] A> (Nos W, X) added. Table 1: <[CJL94] XA> (Nos XA-XB).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FHS2002]
[FHS2002]	(Fukuda+Hanawa+Sugitani, 2002) (Not yet in Simbad)
Write:	<<[FHS2002] Core a>> <<[FHS2002] Peak a>>
N:	4+4
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Note:	C18O cores and 27mm continuum peaks in pillars in the Eagle Nebula. See also EGG, [PAB98], [STN2002].
in source:	M 16 = Eagle Nebula = NGC 6611
Ref:	=2002ApJ...568L.127F
by	FUKUDA N. , HANAWA T., SUGITANI K.
	Astrophys. J., 568, 127-130 (2002)
	Linear sequences of starless cores and young stellar objects in the Eagle nebula.
o	Table 1: <[FHS2002] Core a> (Nos a-d), <[FHS2002] Peak a> (Nos v-y).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FHT2015]
[FHT2015]	(Fukui+Harada+Tokuda+, 2015)
Write:	<<[FHT2015] N159W-W>>
N:	2
Object:	CO Clump (SIMBAD class: MolCld = Molecular Cloud)
Note:	ALMA 13CO(2-1) observations of N=2 CO clumps in the active star-forming region LHA 120-N 159W in the Large Magellanic Cloud.
in source:	Magellanic Clouds:LMC:LHA 120-N 159W = LHA 120-N 159W
Ref:	=2015ApJ...807L...4F
by	FUKUI Y. , HARADA R., TOKUDA K., MORIOKA Y., ONISHI T., TORII K., OHAMA A., HATTORI Y., NAYAK O., MEIXNER M., SEWILO M., INDEBETOUW R., KAWAMURA A., SAIGO K., YAMAMOTO H., TACHIHARA K., MINAMIDANI T., INOUE T., MADDEN S., GALAMETZ M., LEBOUTEILLER V., MIZUNO N., CHEN C.-H.R.
	Astrophys. J., 807L, 4 (2015)
	High-mass star formation triggered by collision between CO filaments in N159 west in the Large Magellanic Cloud.
o	Fig. 1: <[FHT2015] N159W-W> (Nos N159W-N, N159W-S).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FHT99]
[FHT99]	(Flores+Hammer+Thuan+, 1999)
====>	Equivalent to: [FHD99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FHW95]
[FHW95]	(Filipovic+Haynes+White+, 1995)= (LMC) = (LMC-B)
Write:	<<[FHW95] LMC BHHMM+DDMM>>
N:	472
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	See also [FJW97] for radio-sources
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1995A&AS..111..311F
by	FILIPOVIC M.D. , HAYNES R.F., WHITE G.L., JONES P.A., KLEIN U., WIELEBINSKI R.
	Astron. Astrophys., Suppl. Ser., 111, 311-332 (1995)
	A radio continuum study of the Magellanic Clouds. IV. Catalogues of radio sources in the Large Magellanic Cloud at 1.40, 2.45, 4.75, 4.85 and 8.55 GHz.
o	Tables 2 to 7: <[FHW95] LMC BHHMM-DDMM> N=468
Ref:	=1996A&AS..120...77F
by	FILIPOVIC M.D. , WHITE G.L., HAYNES R.F., JONES P.A., MEINERT D., WIELEBINSKI R., KLEIN U.
	Astron. Astrophys., Suppl. Ser., 120, 77-81 (1996)
	A radio continuum study of the Magellanic Clouds. IVa. Catalogue of radio sources in the Large Magellanic Cloud at 2.30GHz (λ=13cm).
o	Table 1: <[FHW95] LMC HHMM+DDMM> N=4 added.
=E=	Catalogue in electronic form as J/A+AS/111/311
=E=	Catalogue in electronic form as J/A+AS/120/77
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FI
FI	(Fitzgerald)
Write:	<<FI NN>>
N:	18
Object:	Poss. G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Ref:	=1974A&A....31..467F
by	FITZGERALD M.P.
	Astron. Astrophys., 31, 467-470 (1974)
	Eighteen possible galaxies in Puppis.
o	<FI NN> (Nos 1-18)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [FI2011]
[FI2011]	(Froebrich+Ioannidis, 2011)
Write:	<<[FI2011] A>> <<[FI2011] MHO NNNN A>>
N:	5+8
Object:	YSO + Outflow (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Molecular outflows and driving sources in [MCM2005b] 14. Use of UKIDSS GPS, UWISH2 and Spitzer IRAC data.
in source:	[MCM2005b] 14
Ref:	=2011MNRAS.418.1375F
by	FROEBRICH D. , IOANNIDIS G.
	Mon. Not. R. Astron. Soc., 418, 1375-1381 (2011)
	About the nature of Mercer 14.
o	Paragr. 3.4: <MHO NNNN> (Nos 2423-2428) added. Table 1: <[FI2011] A> (Nos A-E). Table 2, Fig. 1: <[FI2011] MHO NNNN A> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FIC2017]
[FIC2017]	(Fu+Isbell+Casey+, 2017)
Write:	<<[FIC2017] JDDD.ddddd+DD.ddddd>> <<[FIC2017] GHH HHMM+DDMM>>
N:	27+39
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA Cycle 6 870µm observations of N=39 sources in the field of N=27 bright Herschel near high-redshift QSOs. Use of archival Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS).
Ref:	=2017ApJ...844..123F
by	FU H. , ISBELL J., CASEY C.M., COORAY A., PROCHASKA J.X., SCOVILLE N., STOCKTON A.
	Astrophys. J., 844, 123-123 (2017)
	The circumgalactic medium of submillimeter galaxies. II. Unobscured QSOs within dusty starbursts and QSO sightlines with impact parameters below 100 kpc.
o	Table 2, col(1): <[FIC2017] GHH HHMM+DDMM> N=27. Table 2: <[FIC2017] JDDD.ddddd+DD.ddddd> N=39.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 1FIG
1FIG	(First Fermi-LAT Inner Galaxy Point Source catalog)
Write:	<<1FIG JHHMM.m+DDMM>>
N:	48
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Fermi LAT observations of N=48 sources toward the Galactic Center, the First Fermi-LAT Inner Galaxy Point Source Catalog (1FIG).
in source:	NAME Gal Center
Ref:	=2016ApJ...819...44A
by	AJELLO M. , ALBERT A., ATWOOD W.B., BARBIELLINI G., BASTIERI D., BECHTOL K., BELLAZZINI R., BISSALDI E., BLANDFORD R.D., BLOOM E.D., BONINO R., BOTTACINI E., BRANDT T.J., BREGEON J., BRUEL P., BUEHLER R., BUSON S., CALIANDRO G.A., CAMERON R.A., CAPUTO R., CARAGIULO M., CARAVEO P.A., CECCHI C., CHEKHTMAN A., CHIANG J., CHIARO G., CIPRINI S., COHEN-TANUGI J., COMINSKY L.R., CONRAD J., CUTINI S., D'AMMANDO F., DE ANGELIS A., DE PALMA F., DESIANTE R., DI VENERE L., DRELL P.S., FAVUZZI C., FERRARA E.C., FUSCO P., GARGANO F., GASPARRINI D., GIGLIETTO N., GIOMMI P., GIORDANO F., GIROLETTI M., GLANZMAN T., GODFREY G., GOMEZ-VARGAS G.A., GRENIER I.A., GUIRIEC S., GUSTAFSSON M., HARDING A.K., HEWITT J.W., HILL A.B., HORAN D., JOGLER T., JOHANNESSON G., JOHNSON A.S., KAMAE T., KARWIN C., KNODLSEDER J., KUSS M., LARSSON S., LATRONICO L., LI J., LI L., LONGO F., LOPARCO F., LOVELLETTE M.N., LUBRANO P., MAGILL J., MALDERA S., MALYSHEV D., MANFREDA A., MAYER M., MAZZIOTTA M.N., MICHELSON P.F., MITTHUMSIRI W., MIZUNO T., MOISEEV A.A., MONZANI M.E., MORSELLI A., MOSKALENKO I.V., MURGIA S., NUSS E., OHNO M., OHSUGI T., OMODEI N., ORLANDO E., ORMES J.F., PANEQUE D., PESCE-ROLLINS M., PIRON F., PIVATO G., PORTER T.A., RAINO S., RANDO R., RAZZANO M., REIMER A., REIMER O., RITZ S., SANCHEZ-CONDE M., SAZ PARKINSON P.M., SGRO C., SISKIND E.J., SMITH D.A., SPADA F., SPANDRE G., SPINELLI P., SUSON D.J., TAJIMA H., TAKAHASHI H., THAYER J.B., TORRES D.F., TOSTI G., TROJA E., UCHIYAMA Y., VIANELLO G., WINER B.L., WOOD K.S., ZAHARIJAS G., ZIMMER S.
	Astrophys. J., 819, 44 (2016)
	Fermi-LAT observations of high-energy γ-ray emission toward the Galactic Center.
o	Tables 3+7: <1FIG JHHMM.m+DDMM> N=48.
=E=	Catalogue in electronic form as <J/ApJ/819/44/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FIGS
FIGS	(Faint Infrared Grism Survey)
Write:	<<FIGS GWN NNNN>>
N:	8645
Object:	G (SIMBAD class: Galaxy)
Note:	The Faint Infrared Grism Survey (FIGS) is a deep Hubble Space Telescope (HST) WFC3/IR slitless spectroscopic survey of four deep fields. Two fields are located in the Great Observatories Origins Deep Survey-North (GOODS-N) area and two fields are located in the Great Observatories Origins Deep Survey-South (GOODS-S) area. One of the southern fields selected is the Hubble Ultra Deep Field. Only the first references citing FIGS sources are listed here.
in source:	NAME GOODS North Field
in source:	NAME GOODS South Field
Ref:	=2018ApJ...856..116P
by	PHARO J. , MALHOTRA S., RHOADS J., RYAN R., TILVI V., PIRZKAL N., FINKELSTEIN S., WINDHORST R., GROGIN N., KOEKEMOER A., ZHENG Z., HATHI N., KIM K., JOSHI B., YANG H., CHRISTENSEN L., CIMATTI A., GARDNER J.P., ZAKAMSKA N., FERRERAS I., HIBON P., PASQUALI A.
	Astrophys. J., 856, 116-116 (2018)
	Spectrophotometric redshifts in the Faint Infrared Grism Survey: finding overdensities of faint galaxies.
o	Table 1: Fields GN1, GN2, GS1 and GS2 are not in SIMBAD.
o	Tables 6-7: <[PMR2018] GWN-N.N> N=24. Tables 8-9: <FIGS GWN NNNN> N=38.
Ref:	=2019ApJ...874..125P
by	PHARO J. , MALHOTRA S., RHOADS J., CHRISTENSEN L., FINKELSTEIN S.L., GROGIN N., HARISH S., JIANG T., KIM K., KOEKEMOER A., PIRZKAL N., SMITH M., YANG H., CIMATTI A., FERRERAS I., HATHI N., HIBON P., MEURER G., OESTLIN G., PASQUALI A., RYAN R., STRAUGHN A., WINDHORST R.
	Astrophys. J., 874, 125-125 (2019)
	Emission-line metallicities from the Faint Infrared Grism Survey and VLT/MUSE.
o	Tables 4-6: <FIGS GWN NNNN> N=61 among (GS1 724-GS1 6865).
Ref:	=2019MNRAS.486.1358F
by	FERRERAS I. , PASQUALI A., PIRZKAL N., PHARO J., MALHOTRA S., RHOADS J., HATHI N., WINDHORST R., CIMATTI A., CHRISTENSEN L., FINKELSTEIN S.L., GROGIN N., JOSHI B., KIM K., KOEKEMOER A., O'CONNELL R., OSTLIN G., ROTHBERG B., RYAN R.
	Mon. Not. R. Astron. Soc., 486, 1358-1376 (2019)
	FIGS: spectral fitting constraints on the star formation history of massive galaxies since the cosmic noon.
o	Tables A1-A3: <FIGS GWN NNNN> N=10+14+27 among (Nos GN1 2083-GN1 2590, GN2 411-GN2 1314, GS1 724-GS1 4272).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FIK97]
[FIK97]	(Franx+Illingworth+Kelson+, 1997)
Write:	<<[FIK97] GN>> <<[FIK97] A>>
N:	2+4
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of the cluster 1E 1358.4+6245 = ClG 1358+62. G1 = lensing galaxy, G2 = companion galaxy. (Nos A-D) are components of the cluster, A and D been images of the lensed galaxy, B and C forming a long red arc.
in source:	ClG 1358+6245 = 1E 1358.4+6245
Ref:	=1997ApJ...486L..75F
by	FRANX M. , ILLINGWORTH G.D., KELSON D.D., VAN DOKKUM P.G., TRAN K.
	Astrophys. J., 486, 75-78 (1997)
	A pair of lensed galaxies at z=4.92 in the field of CL 1358+62.
o	Plate L6: Arcs and features format 'A' not in SIMBAD
o	<[FIK97] GN> (Nos G1-G2). <[FIK97] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FIM2015]
[FIM2015]	(Fitzgerald+Inwood+McKinnon+, 2015) (Not yet in Simbad)
Write:	<<[FIM2015] NNN>>
N:	415
Object:	* (SIMBAD class: Star)
Note:	Faulkes Telescope North UBVRI observations of N=415 stars in the field of the open cluster NGC 2215.
in source:	NGC 2215
Ref:	=2015AJ....149..190F
by	FITZGERALD M.T. , INWOOD L., McKINNON D.H., DIAS W.S., SACCHI M., SCOTT B., ZOLINSKI M., DANAIA L., EDWARDS R.
	Astron. J., 149, 190 (2015)
	Photometric and proper motion study of the neglected open cluster NGC 2215.
o	Table 3: <[FIM2015] NNN> (Nos 1-415).
=E=	Catalogue in electronic form as J/AJ/149/190
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FIP2001]
[FIP2001]	(Fricke+Izotov+Papaderos+, 2001)
Write:	<<[FIP2001] GN>> <<[FIP2001] Tol 1214-277 a>> <<[FIP2001] Tol 1214-277 Shell>>
N:	3+2+1
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Note:	VLT FORS1 observations. Fig1(a): N=3 galaxies observed in B-band. Fig1(b): N=2 luminous knots a and b or star-forming regions and N=1 shell observed in R-band in Tol 1214-277
in source:	Tol 1214-277
Ref:	=2001AJ....121..169F
by	FRICKE K.J. , IZOTOV Y.I., PAPADEROS P., GUSEVA N.G., THUAN T.X.
	Astron. J., 121, 169-181 (2001)
	An imaging and spectroscopic study of the very metal-deficient blue compact dwarf galaxy Tol 1214-277.
o	Fig1(a): <[FIP2001] GN> (Nos G1-G3). Fig1(b): <[FIP2001] Tol 1214-277 a> (Nos a-b), <[FIP2001] Tol 1214-277 Shell> N=1.
=E=	Catalogue in electronic form as J/AJ/121/169
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FIR
FIR	(Far IR)
*****	Avoid the usage of FIR, prefer [CEF84]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FIR
FIR	(Far IR)
*****	Avoid the usage of FIR, prefer [CGC93]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FIR
FIR	(Far IR)
*****	Avoid the usage of FIR, prefer [CHT80]
Origin	of the Acronym: A (1991MNRAS.248..670W)
Details on Acronym: FIR
FIR	(Far IR)
*****	Avoid the usage of FIR, prefer [GBM93]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: FIR
FIR	(Far IR)
*****	Avoid the usage of FIR, prefer [HPS93]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FIR
FIR	(Far IR)
*****	Avoid the usage of FIR, prefer [JSP95]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FIR
FIR	(Far IR)
*****	Avoid the usage of FIR, prefer [KLT2003]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FIR
FIR	(Far IR)
*****	Avoid the usage of FIR, prefer [LML2003]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FIR
FIR	(Far IR)
*****	Avoid the usage of FIR, prefer [MCK88]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FIR
FIR	(Far IR)
*****	Avoid the usage of FIR, prefer MFSW
Origin	of the Acronym: L (1989ApJS...69...99S)
Details on Acronym: FIR
FIR	(Far IR)
*****	Avoid the usage of FIR, prefer [MWZ90]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FIR
FIR	(Far IR)
*****	Avoid the usage of FIR, prefer [OF84]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: FIR
FIR	(Far IR)
*****	Avoid the usage of FIR, prefer [SBF2003]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FIR
FIR	(Far IR)
*****	Avoid the usage of FIR, prefer [SHM89]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FIRBACK
FIRBACK	(Far IR Background survey)= (FB)
Write:	<<FIRBACK FSM NN>> <<FIRBACK FNN NN>> <<FIRBACK CFSM NN>> <<FIRBACK CFNN NNN>>
N:	23+56+27+16+47+28
Object:	(FIR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	ISO FIRBACK (Far IR Background) survey. Observations of 3 fields: FSM (FIRBACK South Mareno), FN1 and FN2 (FIRBACK North 1 and 2), with 3 complementary catalogs (CFSM, CFN1 and 2). See also [CSI2002], [PDL2003].
Ref:	=2001A&A...372..364D
by	DOLE H. , GISPERT R., LAGACHE G., PUGET J.-L., BOUCHET F.R., CESARSKY C., CILIEGI P., CLEMENTS D.L., DENNEFELD M., DESERT F.-X., ELBAZ D., FRANCESCHINI A., GUIDERDONI B., HARWIT M., LEMKE D., MOORWOOD A.F.M., OLIVER S., REACH W.T., ROWAN-ROBINSON M., STICKEL M.
	Astron. Astrophys., 372, 364-376 (2001)
	FIRBACK: III. Catalog, source counts, and cosmological implications of the 170 µm ISO deep survey.
o	Table 7: <FIRBACK FSM NN> (Nos 0-22). Table 10: <FIRBACK CFSM NN> (Nos 23-37). Table 8: <FIRBACK FN1 NN> (Nos 0-55). Table 11: <FIRBACK CFN1 NNN> (Nos 56-102). Table 9: <FIRBACK FN2 NN> (Nos 0-26). Table 12: <FIRBACK CFN2 NN> (Nos 27-54).
Ref:	=2003A&A...412..349P
by	PATRIS J. , DENNEFELD M., LAGACHE G., DOLE H.
	Astron. Astrophys., 412, 349-371 (2003)
	Spectroscopic follow-up of FIRBACK-South bright galaxies.
o	Table 2: FSM NNNA, B: partition of IR emission, not in SIMBAD.
o	Table 1: <FIRBACK CFSM NN> (No. 39) added (No. 38 missing). Table 2, Figs: <[PDL2003] FSM NNN N>, <[PDL2003] CFSM NNN N>, N=31.
=E=	Catalogue in electronic form as J/A+A/372/364
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FIRES
FIRES	(Faint IR Extragalactic Survey)
Note:	NIR imaging of the HDFS with ISAAC on VLT, combined with
*****	Avoid the usage of FIRES, prefer [LFR2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FIRS
FIRS	(Far IR Source)
*****	Avoid the usage of FIRS, prefer [CEF84]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FIRS
FIRS	(Far IR Source)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FIRS
FIRS	(Far IR Source)
*****	Avoid the usage of FIRS, prefer [HWJ84]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FIRS
FIRS	(Far IR Source)
*****	Avoid the usage of FIRS, prefer MFSW
Origin	of the Acronym: L (1982ApJ...258..165F)
Details on Acronym: FIRST
FIRST	(Faint Images of the Radio Sky at Twenty-cm)= (FRS)
Write:	<<FIRST JHHMMSS.s+DDMMSS>>
N:	236040+946432
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	FIRST survey produces the radio equivalent (at 20 cm) of the Palomar Observatory Sky Survey over 10000 square degrees of the North Galactic Cap. Using the NRAO Very Large Array (VLA) and an automated mapping pipeline, images are produced with 1.8" pixels, a typical rms of 0.15mJy, and a resolution of 5". At the 1mJy source detection threshold, there are 90 sources per square degree, 35per100 of which have resolved structure on scales from 2-20". The FIRST survey is described in Becker+ 1995ApJ...450..559B, and more details are given in 1997ApJ....475..479W. The final version of the catalog is described in 2015ApJ...801...26H. Format of objects in the catalogue is 'HHMMSS.sss+DDMMSS.ss', since the actual accuracy of the positions requires this precision, but the authors used the format 'HHMMSS.s+DDMMSS' for designation.
Ref:	=1997ApJ...475..479W
by	WHITE R.L. , BECKER R.H., HELFAND D.J., GREGG M.D.
	Astrophys. J., 475, 479-493 (1997)
	A catalog of 1.4 GHz radio sources from the FIRST survey.
o	<FIRST JHHMMSS.s+DDMMSS> N=138664
Ref:	=2015ApJ...801...26H
by	HELFAND D.J. , WHITE R.L., BECKER R.H.
	Astrophys. J., 801, 26 (2015)
	The last of FIRST: the final catalog and source identifications.
o	<FIRST JHHMMSS.s+DDMMSS> N=946432.
=E=	Catalogue in electronic form as <VIII/59/>
=E=	Catalogue in electronic form as <VIII/71/>
=E=	Catalogue in electronic form as <VIII/90/>
=E=	Catalogue in electronic form as <VIII/92/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FIRST-BNGS
FIRST-BNGS	(FIRST-Bright Natural Guide Star)
Write:	<<FIRST-BNGS JHHMM+DDMMWW>> <<FIRST-BNGS FHHMM+DDMMWW>> (not recognised by Simbad, but found in literature)
N:	64
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA FIRST sources with a bright nearby star. UH2.2m and WIYN optical photometry, CFHT and Subaru IRCS NIR photometry, IRTF SpeX, Gemini GMOS and Keck II OSIRIS spectroscopy.
Ref:	=2009ApJS..185..124S
by	STALDER B. , CHAMBERS K.C., VACCA W.D.
	Astrophys. J., Suppl. Ser., 185, 124-155 (2009)
	58 radio sources near bright natural guide stars.
o	Table 1: <FIRST-BNGS JHHMM+DDMMWW> N=64.
=E=	Catalogue in electronic form as J/ApJS/185/124
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FJ
FJ	(Finlay+Jones) (Not yet in Simbad)
*****	Avoid the usage of FJ, prefer [FJ73]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [FJ73]
[FJ73]	(Finlay+Jones, 1973)= (FJ) = (FRO) (Not yet in Simbad)
Write:	<<[FJ73] HHMM+DD>>
N:	175
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1973AuJPh..26..389F
by	FINLAY E.A. , JONES B.B.
	Australian J. Phys., 26, 389-402 (1973)
	Measurements of source strengths at 29.9 MHz.
o	Table 2: <[FJ73] HHMM+DD> N=175
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FJ78]
[FJ78]	(Ford+Jacoby, 1978)
*****	Avoid the usage of [FJ78], prefer Ford
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FJ95]
[FJ95]	(Fabricius+Jorgensen, 1995)
Write:	<<[FJ95] NN>>
N:	54
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Identif. charts
Ref:	=1995A&A...296L...1F
by	FABRICIUS C. , JOERGENSEN H.E.
	Astron. Astrophys., 296, 1-4 (1995)
	An astrometric grid for the centre of the Galaxy.
o	Table 1: <[FJ95] NN> N=54
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FJ97]
[FJ97]	(Fabbiano+Juda, 1997)
Write:	<<[FJ97] N>>
N:	8
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations
in source:	NGC 4594 = M 104 = Sombrero Galaxy
Ref:	=1997ApJ...476..666F
by	FABBIANO G. , JUDA J.Z.
	Astrophys. J., 476, 666-676 (1997)
	ROSAT observations of the Sombrero galaxy: discovery of an X-ray active nucleus.
o	Table 2: <[FJ97] N> (Nos 1-8)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FJB2011]
[FJB2011]	(Foster+Jackson+Barnes+, 2011)
Write:	<<[FJB2011] GLLL.lll+BB.bbb>>
N:	182
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	Mopra 22m radio telescope spectroscopy at 90GHz of N=182 candidate dense molecular clumps, in preparation for the Millimeter Astronomy Legacy Team Survey at 90GHz (MALT90).
Ref:	=2011ApJS..197...25F
by	FOSTER J.B. , JACKSON J.M., BARNES P.J., BARRIS E., BROOKS K., CUNNINGHAM M., FINN S.C., FULLER G.A., LONGMORE S.N., MASCOOP J.L., PERETTO N., RATHBORNE J., SANHUEZA P., SCHULLER F., WYROWSKI F.
	Astrophys. J., Suppl. Ser., 197, 25 (2011)
	The Millimeter Astronomy Legacy Team 90 GHz (MALT90) pilot survey.
o	Tables 3-5: <[FJB2011] GLLL.lll+BB.bbb> N=182.
=E=	Catalogue in electronic form as J/ApJS/197/25
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FJCHP
FJCHP	(Ford+Jacoby+Ciardullo+Hui+Ptak)
Write:	<<NAME FJCHP NN>>
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	PNs from a list of Ford+ not published.
Ref:	=1999ApJ...515..169J
by	JACOBY G.H. , CIARDULLO R.
	Astrophys. J., 515, 169-190 (1999)
	Chemical abundances of planetary nebulae in the bulge and disk of M31.
o	Table 1: objects CJFN are Ford M 31 NNN in SIMBAD.
o	Table 1: <NAME FJCHP NN> (Nos 51, 57, 58).
Origin	of the Acronym: L (1999ApJ...515..169J)
Details on Acronym: [FJD2019]
[FJD2019]	(Francis+Johnstone+Dunham+, 2019)
Write:	<<[FJD2019] NN>>
N:	22
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA 1.3mm observations of N=22 sources in the Serpens molecular cloud.
in source:	NAME Serpens Cloud
Ref:	=2019ApJ...871..149F
by	FRANCIS L. , JOHNSTONE D., DUNHAM M.M., HUNTER T.R., MAIRS S.
	Astrophys. J., 871, 149-149 (2019)
	Identifying Variability in deeply embedded protostars with ALMA and CARMA.
o	Figs 2-3, Table 5: <[FJD2019] NN> (Nos 1-22).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FJF
FJF	(F.J. Fuenmayor)
*****	Avoid the usage of FJF, prefer Fuen
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [FJH2005]
[FJH2005]	(Fynbo+Jensen+Hjorth+, 2005)
Write:	<<[FJH2005] GRB 050401 abs N.NN>>
N:	2
Object:	Absorber
Note:	FORS2 VLT observations of GRB 050401.
Ref:	=2005GCN..3176....1F
by	FYNBO J.P.U. , JENSEN B.L., HJORTH J., WIERSEMA K., STARLING R., VREESWIJK P., ROL E., LEVAN A., ELLISON S., MASETTI N.
	GRB Coordinates Network, Circular Service, 3176, 1-None (2005)
	GRB 050401: VLT spectroscopic redshift.
o	<[FJH2005] GRB 050401 abs N.NN> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FJJ
FJJ	(Ford+Jacoby+Jenner)
Write:	<<FJJ NGC 147 N>> <<FJJ NGC 147 a>> <<FJJ NGC 147 R>> <<FJJ NGC 185 N>> <<FJJ NGC 185 a>> <<FJJ NGC 185 R>>
N:	5+6+4+5+7+8
Object:	Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 2: format 'NGC 147 N', N=5 PN, format 'NGC 147 a', N=6 ref. * (Nos a-f). Table 3: format 'NGC 185 N', N=5 PN, format 'NGC 185 a', N=7 ref. * (Nos a-g). Table 9: format 'NGC 185 R', N=8 GCl (Nos I-VIII), format 'NGC 147 R', N=4 GCl (Nos I-IV). see also Ford
in source:	NGC 185
in source:	NGC 147
Ref:	=1977ApJ...213...18F
by	FORD H.C. , JACOBY G., JENNER D.C.
	Astrophys. J., 213, 18-26 (1977)
	Planetary nebulae in local group galaxies. IV. Identifications, positions and radial velocities of nebulae in NGC 147 and NGC 185.
o	FJJ NGC 185 g NOT = AGK3 +48 660 in SIMBAD
o	Table 2: <FJJ NGC 147 N> N=5, <FJJ NGC 147 a> N=6. Table 3: <FJJ NGC 185 N> N=5, <FJJ NGC 185 a> N=7. Table 9: <FJJ NGC 185 R> N=8, <FJJ NGC 147 R> N=4
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [FJL2017]
[FJL2017]	(Feher+Juvela+Lunttila+, 2017)
Write:	<<[FJL2017] GLLL.ll+BB.bbA>> <<[FJL2017] GLLL.ll+BB.bb-1A>>
N:	35
Object:	Clump (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	OSO 20-m telescope 12CO(1-0) and 13CO(1-0) line observations of N=35 high-density clumps in N=26 Herschel fields.
Ref:	=2017A&A...606A.102F
by	FEHER O. , JUVELA M., LUNTTILA T., MONTILLAUD J., RISTORCELLI I., ZAHORECZ S., TOTH L.V.
	Astron. Astrophys., 606A, 102-102 (2017)
	A CO survey on a sample of Herschel cold clumps.
o	Tables 1-2: <[FJL2017] GLLL.ll+BB.bb A>, [FJL2017] GLLL.ll+BB.bb-1A> N=35.
=E=	Catalogue in electronic form as J/A+A/606/A102
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FJM
FJM	(Furniss+Jennings+Moorwood)
Write:	<<FJM N>>
N:	6
Object:	(Far IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Ref:	=1972ApJ...176L.105F
by	FURNISS I. , JENNINGS R.E., MOORWOOD A.F.M.
	Astrophys. J., 176, 105-108 (1972)
	Detection of far-infrared astronomical sources.
o	Table 1: <FJM N> (Nos 1-6)
Origin	of the Acronym: L (1979AJ.....84.1574F)
Details on Acronym: [FJM2003]
[FJM2003]	(Fynbo+Jakobsson+Moller+, 2003)
Write:	<<[FJM2003] SMMDD-N>>
N:	7
Object:	Em. Obj. (SIMBAD class: EmObj = Emission Object)
Stat:	is completely incorporated in Simbad
Note:	NTT SUSI2 observations. N=7 candidate LEGOs (Ly-alpha Emitting Galaxy-building Object) in the field of GRB 011211 (1211 in the format). See also [FMT2002], [JBF2005], LEGO.
Ref:	=2003A&A...406L..63F
by	FYNBO J.P.U. , JAKOBSSON P., MOLLER P., HJORTH J., THOMSEN B., ANDERSEN M.I., FRUCHTER A.S., GOROSABEL J., HOLLAND S.T., LEDOUX C., PEDERSEN H., RHOADS J., WEIDINGER M., WIJERS R.A.M.J.
	Astron. Astrophys., 406, 63-66 (2003)
	On the Lyα emission from γ-ray burst host galaxies: Evidence for low metallicities.
o	Table 1: <[FJM2003] S1211-N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FJP2007]
[FJP2007]	(Feldmeier+Jacoby+Phillips, 2007)
Write:	<<[FJP2007] NGC NNNN NN>>
N:	45+44+94
Object:	Poss. PN (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
Note:	Magellan Clay and WIYN 3.5m telescope observations. Search for PN in 3 galaxies.
in source:	NGC 1316 = For A
in source:	NGC 1380
in source:	NGC 4526
Ref:	=2007ApJ...657...76F
by	FELDMEIER J.J. , JACOBY G.H., PHILLIPS M.M.
	Astrophys. J., 657, 76-94 (2007)
	Calibrating type Ia supernovae using the planetary nebula luminosity function. I. Initial results.
o	Table 3: <[FJP2007] NGC 1316 NN> (Nos 1-45). Table 4: <[FJP2007] NGC 1380 NN> (Nos 1-44). Table 5: <[FJP2007] NGC 4526 NN> (Nos 1-94).
=E=	Catalogue in electronic form as J/ApJ/657/76
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FJS2005]
[FJS2005]	(Fynbo+Jensen = Sollerman+, 2005)
Write:	<<[FJS2005] GRB 050824 abs N.NN>>
N:	1
Object:	Absorber
Note:	ESO VLT FORS2 observations.
Ref:	=2005GCN..3874....1F
by	FYNBO J.P.U. , JENSEN B.L., SOLLERMAN J., HJORTH J., WATSON D., PEDERSEN K., JAKOBSSON P., CASTRO CERON J.M., GOROSABEL J.
	GRB Coordinates Network, Circular Service, 3874, 1-None (2005)
	GRB 050824: spectroscopic redshift from the VLT.
o	<[FJS2005] GRB 050824 abs N.NN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FJS2008]
[FJS2008]	(Fuentes-Carrera+Jablonka+Sarajedini+, 2008)
Write:	<<[FJS2008] GNNN NNNNNN>>
N:	8805+15233+12982
Object:	*inCl (SIMBAD class: Star)
Note:	HST ACS observations of N=3 massive clusters in M 31.
in source:	M 31 = NGC 224:SKHB 78 = SKHB 78
in source:	M 31 = NGC 224:SKHB 213 = SKHB 213
in source:	M 31 = NGC 224:SKHB 280 = SKHB 280
Ref:	=2008A&A...483..769F
by	FUENTES-CARRERA I. , JABLONKA P., SARAJEDINI A., BRIDGES T., DJORGOVSKI G., MEYLAN G.
	Astron. Astrophys., 483, 769-781 (2008)
	Evidence for metallicity spreads in three massive M31 globular clusters.
o	Paragraph 2.1 : objects D68 and D642 = [H80] 68 and [H80] 642 in Simbad.
o	Table 2a: <[FJS2008] G78 NNNNNN> N=8805. Table 2b: <[FJS2008] G213 NNNNNN> N=15233. Table 2c: <[FJS2008] G280 NNNNNN> N=12982.
=E=	Catalogue in electronic form as J/A+A/483/769
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FJS82]
[FJS82]	(Fischer+Joyce+Simon, 1982) (Not yet in Simbad)
Write:	<<[FJS82] IRS V-N>>
N:	3
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Superseded by [SDW85]
in source:	NGC 6334:MFSW V = MFSW V
Ref:	=1982ApJ...258..165F
by	FISCHER J. , JOYCE R.R., SIMON M., SIMON T.
	Astrophys. J., 258, 165-169 (1982)
	Near-infrared observations of the far-infrared source V region in NGC 6334.
o	[FJS82] superseded by <[SDW85] IRS V-N> (Nos V-1 to V-3)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FJW97]
[FJW97]	(Filipovic+Jones+White+, 1997)= (SMC)
Write:	<<[FJW97] SMC BHHMM+DDMM>>
N:	224
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	See also [FHW95] for radio-sources in the LMC
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1997A&AS..121..321F
by	FILIPOVIC M.D. , JONES P.A., WHITE G.L., HAYNES R.F., KLEIN U., WIELEBINSKI R.
	Astron. Astrophys., Suppl. Ser., 121, 321-326 (1997)
	A radio continuum study of the Magellanic Clouds. V. Catalogues of radio sources in the Small Magellanic Cloud at 1.42, 2.45, 4.75, 4.85 and 8.55 GHz.
o	Tables 1-6: <[FJW97] SMC BHHMM-DDMM> N=224
=E=	Catalogue in electronic form as J/A+AS/121/321
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FK
FK	(Fesen+Kirshner) (Not yet in Simbad)
*****	Avoid the usage of FK, prefer [FK82]
Origin	of the Acronym: L (2010ApJ...716L...9L)
Details on Acronym: FK
FK	(Feigelson+Kriss)
*****	Avoid the usage of FK, prefer [FK81]
Origin	of the Acronym: L (1983ApJ...269..229M)
Details on Acronym: FK
FK	(Feigelson+Kriss)
*****	Avoid the usage of FK, prefer [FK83]
Origin	of the Acronym: L (1985AJ.....90.1490V)
Details on Acronym: FK 4
FK 4	(Fundamental Katalog, 4th)
*****	Avoid the usage of FK 4, prefer FK5
Details on Acronym: FK/4
FK/4	(Fundamental Katalog, 4th)
====>	Equivalent to: FK5
Details on Acronym: [FK2002]
[FK2002]	(Focardi+Kelm, 2002)= (UZC-CG)
Write:	<<[FK2002] NNN>>
N:	291
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=291 compact groups from the UZC catalogue. See also galaxies in each group, [FK2002] NNNa.
Ref:	=2002A&A...391...35F
by	FOCARDI P. , KELM B.
	Astron. Astrophys., 391, 35-46 (2002)
	Compact groups in the UZC galaxy sample.
o	Table 1: <[FK2002] NNN> (Nos 1-291).
=E=	Catalogue in electronic form as J/A+A/391/35
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FK2002]
[FK2002]	(Focardi+Kelm, 2002)= (UZC-CG)
Write:	<<[FK2002] NNNa>>
N:	986
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Note:	Galaxy members for each [FK2002] NNN group. These galaxies are found in 2002A&A...391...35F, table 2, but later designated similarly to HCG with a format NNNa.
Ref:	=2008ApJ...678L...9M
by	MARTINEZ M.A. , DEL OLMO A., COZIOL R., FOCARDI P.
	Astrophys. J., 678L, 9-12 (2008)
	Deficiency of broad-line AGNs in compact groups of galaxies.
o	Table 1: <[FK2002] NNNa> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FK2005]
[FK2005]	(Feng+Kaaret, 2005)
Write:	<<[FK2005] NN>>
Object:	ULX (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of ULXs in nearby galaxies.
Ref:	=2005ApJ...633.1052F
by	FENG H. , KAARET P.
	Astrophys. J., 633, 1052-1063 (2005)
	XMM-Newton observations of ultraluminous X-ray sources in nearby galaxies.
o	Table 2: <[FK2005] NN> (Nos 1-28).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FK2008]
[FK2008]	(Feng+Kaaret, 2008)
Write:	<<[FK2008] source N>> <<[FK2008] star A>>
N:	2+2
Object:	(X) + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Chandra and HST observation of ULX [FT87] IC 342 1.
Ref:	=2008ApJ...675.1067F
by	FENG H. , KAARET P.
	Astrophys. J., 675, 1067-1075 (2008)
	Optical counterpart of the ultraluminous X-ray source IC 342 X-1.
o	IC 342 X-1 = [FT87] IC 342 1 in SIMBAD.
o	Fig.1, Table 1: <[FK2008] source N> (Nos 1-2). Fig.2: <[FK2008] star A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FK3
FK3	(Fundamental Katalog. 3rd)
====>	Equivalent to: FK5
Details on Acronym: FK4
FK4	(Fundamental Katalog, 4th)
Note:	Revision of FK3, includes FK3 Suppl.
====>	Equivalent to: FK5
Details on Acronym: FK5
FK5	(Fundamental Katalog, 5th)= FK3 = FK4 = (FK 4) = FK/4
Write:	<<FK5 NNNN>>
N:	5647
Object:	* (SIMBAD class: Star)
Note:	Basic FK5, Revision of the FK4 catalogue. The catalogue provides, improved mean positions and proper motions for classical fundamental stars which were already included in the FK3 and FK4 and mean positions and proper motions for new fundamental stars extending also the fundamental system to the apparent magnitude 9.5. The assignement of numbers to stars is the same as in the FK4, the data are given in the order of right ascension for equinox and epoch J2000.0. Among (Nos 1-905) and (Nos 1001-1670), 52 stars are no longer regarded as fundamental and are missing in the series 1-905. New: (Nos 2003-6125).
Ref:	=1988VeARI..32....1F
by	FRICKE W. , SCHWAN H., LEDERLE T.
	Veroeff. Astron. Rechen-Inst. Heidelberg, 32, 1-106 (1988)
	Fifth fundamental catalogue.
o	<FK5 NNNN> N=873 among (Nos 1-925) + N=662 among (Nos 1001-1630)
Ref:	=1991VeARI..33....1F
by	FRICKE W. , SCHWAN H., CORBIN T., BASTIAN U., BIEN R., COLE C., JACKSON R., JAEHRLING R., JAHREISS H., LEDERLE T.
	Veroeff. Astron. Rechen-Inst. Heidelberg, 33, 1-None (1991)
	Fifth Fundamental Catalogue (FK5) Part II. The FK5 extension.
o	<FK5 NNNN> (Nos 2003-6125)
=E=	Catalogue in electronic form as I/149
=E=	Catalogue in electronic form as I/175
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FK6
FK6	(Fundamental Katalog, 6th)
Write:	<<FK5 NNNN>>
Object:	* (SIMBAD class: Star)
Note:	The FK6 is a suitable combination of the results of the HIPPARCOS astrometry satellite with ground-based data summarized in the FK5. Same numbering as in the FK5 catalogue.
Ref:	=1999VeARI..35....1W
by	WIELEN R. , SCHWAN H., DETTBARN C., LENHARDT H., JAHREISS H., JAHRLING R.
	Veroeff. Astron. Rechen-Inst. Heidelberg, 35, 1-None (1999)
	Sixth catalogue of fundamental stars (FK6). Part I. Basic fundamental stars with direct solutions.
o	FK6 NNNN, same numbering as FK5, use <FK5 NNNN> N=4150.
Ref:	=2000VeARI..37....1W
by	WIELEN R. , SCHWAN H., DETTBARN C., LENHARDT H., JAHREISS H., JAHRLING R., KHALISI E.
	Veroeff. Astron. Rechen-Inst. Heidelberg, 37, 1-None (2000)
	Sixth catalogue of fundamental stars (FK6). Part III. Additional stars with direct solutions.
o	FK6 NNNN, same numbering as FK5, use <FK5 NNNN> N=4150.
=E=	Catalogue in electronic form as I/264
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FK81]
[FK81]	(Feigelson+Kriss, 1981)= (FK)
Write:	<<[FK81] N>>
N:	3
Object:	Pre Main Seq. * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1981ApJ...248L..35F
by	FEIGELSON E.D. , KRISS G.A.
	Astrophys. J., 248, 35-38 (1981)
	Discovery of three X-ray luminous pre-main-sequence stars.
o	Table 1: <[FK81] N> (Nos 1-3)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FK82]
[FK82]	(Fesen+Kirshner, 1982)= (FK) (Not yet in Simbad)
Write:	<<[FK82] NN>>
N:	10
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Kitt Peak 1.3m McGraw-Hill spectrophotometry at N=10 locations in the Crab Nebula filaments.
in source:	NGC 1952
Ref:	=1982ApJ...258....1F
by	FESEN R.A. , KIRSHNER R.P.
	Astrophys. J., 258, 1-10 (1982)
	The Crab Nebula. I. Spectrophotometry of the filaments.
o	Fig. 1, Table 1: <[FK82] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FK83]
[FK83]	(Feigelson+Kriss, 1983)= (FK)
Write:	<<[FK83] LDN NNNN NNA>> <<[FK83] LkHA 120 NN>>
N:	71+40+48+22
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	LDN 1551
in source:	LDN 1544
in source:	LDN 1529
in source:	EM* LkHA 120
Ref:	=1983AJ.....88..431F
by	FEIGELSON E.D. , KRISS G.A.
	Astron. J., 88, 431-438 (1983)
	A search for weak H-α emission line pre-main-sequence stars.
o	Table II: <[FK83] LDN 1551 NNA> N=71, <[FK83] LDN 1544 NN> N=40, <[FK83] LDN 1529 NN> N=48, <[FK83] LkHA 120 NN> N=22.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKA2008]
[FKA2008]	(Fassnacht+Kocevski+Auger+, 2008)
Write:	<<[FKA2008] B2108>> <<[FKA2008] B2108-N>>
N:	3
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	Chandra observations of galaxy groups.
Ref:	=2008ApJ...681.1017F
by	FASSNACHT C.D. , KOCEVSKI D.D., AUGER M.W., LUBIN L.M., NEUREUTHER J.L., JELTEMA T.E., MULCHAEY J.S., McKEAN J.P.
	Astrophys. J., 681, 1017-1034 (2008)
	The X-ray properties of moderate-redshift galaxy groups selected by association with gravitational lenses.
o	Table 2, Text: <[FKA2008] B2108-N> (Nos 1-2). Text: <[FKA2008] B2108> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKB99]
[FKB99]	(Frail+Kulkarni+Bloom+, 1999)= (VLA)
Write:	<<[FKB99] VLA JHHMMSS.s+DDMMSS>> <<[FKB99] Star A>> <<[FKB99] JHHMMSS.ss+DDMMSS.ss>>
N:	2+1+1
Object:	(Rad) + * + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=1 VLA transient coincident with the proposed X-ray afterglow for the gamma-ray burst GRB 981226: 'VLA J232937.2-235553', and N=1 other comparison VLA: 'VLA J232940.0-235254'. N=1 star in Fig.3: 'Star A'. N=1 extended object, 'J232936.11-235553.41' proposed to be the host galaxy of the GRB.
Ref:	=1999ApJ...525L..81F
by	FRAIL D.A. , KULKARNI S.R., BLOOM J.S., DJORGOVSKI S.G., GORJIAN V., GAL R.R., MELTZER J., SARI R., CHAFFEE F.H., GOODRICH R., FRONTERA F., COSTA E.
	Astrophys. J., 525, 81-84 (1999)
	The radio afterglow and the host galaxy of the X-ray-rich GRB 981226.
o	<[FKB99] VLA JHHMMSS.s+DDMMSS> N=2. <[FKB99] Star A> (No. A). <[FKB99] JHHMMSS.ss+DDMMSS.ss> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKC2006]
[FKC2006]	(Fomalont+Kellermann+Cowie+, 2003)
Write:	<<[FKC2006] NNNA>> <<[FKC2006] NNNNA>>
N:	810+68
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA at 1.4GHz observations of the Hawaii SSA 13 field: Radio-optical catalog of 810 sources. The letter N before the number indicates that it is not in the complete sample of 560 sources. The letter A, B, etc, at the end of the format stands for components of the same source.
Ref:	=2006ApJS..167..103F
by	FOMALONT E.B. , KELLERMANN K.I., COWIE L.L., CAPAK P., BARGER A.J., PARTRIDGE R.B., WINDHORST R.A., RICHARDS E.A.
	Astrophys. J., Suppl. Ser., 167, 103-160 (2006)
	The Radio/Optical catalog of the SSA 13 field.
o	Table 2: <[FKC2006] NNN> N=560 among (Nos 9-797), <[FKC2006] ANNN> N=250 among (Nos N001-N810), <[FKC2006] NNNA>, <[FKC2006] ANNNA>, N=68.
=E=	Catalogue in electronic form as J/ApJS/167/103
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKC2008]
[FKC2008]	(Faure+Kneib+Covone+, 2008)= (COSMOS)
Write:	<<[FKC2008] COSMOS MMSS+MMSS>> <<[FKC2008] COSMOS MMSS+MMSS lens>> <<[FKC2008] COSMOS MMSS+MMSS source>>
N:	67+67+67
Object:	Grav. lens system + Grav. lens + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=67 strong lens candidates in the COSMOS field. Use of HST ACS, Subaru Suprime camera, and CFHT Megacam data.
in source:	NAME COSMOS Field
Ref:	=2008ApJS..176...19F
by	FAURE C. , KNEIB J.-P., COVONE G., TASCA L., LEAUTHAUD A., CAPAK P., JAHNKE K., SMOLCIC V., DE LA TORRE S., ELLIS R., FINOGUENOV A., KOEKEMOER A., LE FEVRE O., MASSEY R., MELLIER Y., REFREGIER A., RHODES J., SCOVILLE N., SCHINNERER E., TAYLOR J., VAN WAERBEKE L., WALCHER J.
	Astrophys. J., Suppl. Ser., 176, 19-38 (2008)
	First catalog of strong lens candidates in the COSMOS field.
o	(Erratum) erratum vol. 178, p. 382 (2008)
o	Tables 1-2: <[FKC2008] COSMOS MMSS+MMSS>, <[FKC2008] COSMOS MMSS+MMSS lens>, <[FKC2008] COSMOS MMSS+MMSS source> N=67+67+67.
=E=	Catalogue in electronic form as J/ApJS/176/19
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKC2012]
[FKC2012]	(Fruth+Kabath+Cabrera+, 2012)= (BEST)
Write:	<<[FKC2012] LRa02a2 NNNNN>>
N:	331+17
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Berlin Exoplanet Search Telescope II (BEST II) observations of the CoRoT LRa02 field. See also [KER2009].
Ref:	=2012AJ....143..140F
by	FRUTH T. , KABATH P., CABRERA J., CHINI R., CSIZMADIA Sz., EIGMULLER P., ERIKSON A., KIRSTE S., LEMKE R., MURPHY M., PASTERNACKI T., RAUER H., TITZ-WEIDER R.
	Astron. J., 143, 140 (2012)
	Improved variable star search in large photometric data sets: new variables in CoRoT field LRa02 detected by BEST II.
o	Tables 3-4: <[FKC2012] LRa02a2 NNNNN> N=331+17 among (Nos LRa02a2 00759 to LRa02a2 44056, LRa02b2 00490 to 76168).
=E=	Catalogue in electronic form as <J/AJ/143/140/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKD2012]
[FKD2012]	(Faundez-Abans+Krabbe+De Oliveira-Abans+, 2012)
Write:	<<[FKD2012] A>> <<[FKD2012] AM546-324>>
N:	5 (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Gemini GMOS-S observations of the field of the system of interacting galaxies 2MASX J05483518-3240006 and 2MFGC 4711.
Ref:	=2012A&A...543A..64F
by	FAUNDEZ-ABANS M. , KRABBE A.C., DE OLIVEIRA-ABANS M., DA ROCHA-POPPE P.C., RODRIGUES I., FERNANDES-MARTIN V.A., FERNANDES I.F.
	Astron. Astrophys., 543A, 64-64 (2012)
	A study of the remarkable galaxy system AM 546-324 (the core of Abell S0546).
o	Table 1, Table 2 : <[FKD2012] A> (Nos P,K,C,S) ; <[FKD2012] AM546-324>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKD2021]
[FKD2021]	(Fogasy+Knudsen+Drouart+, 2021)
Write:	<<[FKD2021] TXS 0828+193 companion #N>>
N:	4
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	ALMA band3 CO(3-2) observations of N=4 potential companions in the halo of the radio galaxy TXS 0828+193.
Ref:	=2021MNRAS.501.5973F
by	FOGASY J. , KNUDSEN K.K., DROUART G., GULLBERG B.
	Mon. Not. R. Astron. Soc., 501, 5973-5980 (2021)
	ALMA detects molecular gas in the halo of the powerful radio galaxy TXS 0828+193.
o	Fig. 3, Table 1: <[FKD2021] TXS 0828+193 companion #N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKG2015]
[FKG2015]	(Fausnaugh+Kochanek+Gerke+, 2015)
Write:	<<[FKG2015] NN>>
N:	81
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Stat:	is completely incorporated in Simbad
Note:	Telescope LBC observations of N=81 Cepheid stars in the maser-host galaxy NGC 4258.
in source:	M 106 = NGC 4258
Ref:	=2015MNRAS.450.3597F
by	FAUSNAUGH M.M. , KOCHANEK C.S., GERKE J.R., MACRI L.M., RIESS A.G., STANEK K.Z.
	Mon. Not. R. Astron. Soc., 450, 3597-3619 (2015)
	The Cepheid distance to the maser-host galaxy NGC 4258: studying systematics with the Large Binocular Telescope.
o	Table 1: <[FKG2015] NN> N=43 (Nos 1-43), Table 2: <[FKG2015] NN> N=38 (Nos 44-81).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKG93]
[FKG93]	(Fabriquant+Kurtz+Geller+, 1993)
Write:	<<[FKG93] HHMMSS.s+DDMMSS>>
N:	350
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table 1: the authors don't give any format to their list, so we use the coordinates as format.
in source:	ACO 119
Ref:	=1993AJ....105..788F
by	FABRICANT D. , KURTZ M., GELLER M., ZABLUDOFF A., MACK P., WEGNER G.
	Astron. J., 105, 788-796 (1993)
	A study of the rich cluster of galaxies A119.
o	col(2): Cross-id No. Dressler [D80] users : [FGK93] 005501.6 -013939 is [D80] ACO 119 26 (not 2) according to D80, ref. MQ seems to quote [D80] ACO 119 2 = [FGK93] 005307.4-015715.
o	Table 1: <[FKG93] HHMMSS.s+DDMMSS> N=350
=E=	Catalogue in electronic form as J/AJ/105/788
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKK2007]
[FKK2007]	(Foster+Kothes+Kerton+, 2007) (Not yet in Simbad)
Write:	<<[FKK2007] IR N>>
N:	2
Object:	(Far IR) (SIMBAD class: FarIR = Far-IR source (λ >= 30 µm))
Note:	Far IR observations in IRAS HIRES images of GAL 084.9+00.5 HII region.
in source:	GAL 084.9+00.5
Ref:	=2007ApJ...667..248F
by	FOSTER T.J. , KOTHES R., KERTON C.R., ARVIDSSON K.
	Astrophys. J., 667, 248-256 (2007)
	Revealing the Galactic H II region G84.9+0.5 through 5 GHz continuum and polarization emission and a Voigt profile analysis of radio recombination line observations.
o	Fig.5: <[FKK2007] IR N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKK2016]
[FKK2016]	(Furusawa+Kashikawa+Kobayashi+, 2016) (Not yet in Simbad)
Write:	<<[FKK2016] FHN-NNNNN>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Note:	Subaru Suprime-Cam photometric observations of N=3 galaxies at z=7 in the UDS field.
Ref:	=2016ApJ...822...46F
by	FURUSAWA H. , KASHIKAWA N., KOBAYASHI M.A.R., DUNLOP J.S., SHIMASAKU K., TAKATA T., SEKIGUCHI K., NAITO Y., FURUSAWA J., OUCHI M., NAKATA F., YASUDA N., OKURA Y., TANIGUCHI Y., YAMADA T., KAJISAWA M., FYNBO J.P.U., FEVRE O.L.
	Astrophys. J., 822, 46-46 (2016)
	A new constraint on the Lyα fraction of UV very bright galaxies at redshift 7.
o	Table 2: <[FKK2016] FHN-NNNNN> N=3 among (Nos FH2-22303 to FH4-42903).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKK89]
[FKK89]	(Fabricant+Kent+Kurtz, 1989)
Write:	<<[FKK89] NNN>>
N:	172
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	ACO 2256
Ref:	=1989ApJ...336...77F
by	FABRICANT D.G. , KENT S.M., KURTZ M.J.
	Astrophys. J., 336, 77-92 (1989)
	A combined optical/X-ray study of the galaxy cluster Abell 2256.
o	Table 1, col(1): <[FKK89] NNN> (Nos 1-172). Table 1, col(8): <[D76] NNN> N=74 among (Nos 14-486).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKM2008]
[FKM2008]	(Fukui+Kawamura+Minamidani+, 2008)= (LMC N)
Write:	<<[FKM2008] NNN>> <<[FKM2008] LMC N JHHMM+DDMM>>
N:	272-268
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	NANTEN 4m radio telescope CO(1-0) observations to search for molecular clouds in the LMC.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2008ApJS..178...56F
by	FUKUI Y. , KAWAMURA A., MINAMIDANI T., MIZUNO Y., KANAI Y., MIZUNO N., ONISHI T., YONEKURA Y., MIZUNO A., OGAWA H., RUBIO M.
	Astrophys. J., Suppl. Ser., 178, 56-70 (2008)
	The second survey of the molecular clouds in the Large Magellanic Cloud by NANTEN. I. Catalog of molecular clouds.
o	Tables 1-2, col(1): <[FKM2008] NNN> (Nos 1-272) = Tables 1-2, col(2): <[FKM2008] LMC N JHHMM+DDMM> N=268.
=E=	Catalogue in electronic form as J/ApJS/178/56
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKN97]
[FKN97]	(Frail+Kulkarni+Nicastro+, 1997)= ([FKN97a]) = (VLA)
Write:	<<[FKN97] JHHMM.m+DDMM>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=4 radio-sources in the errorbox of GRB 970111. The authors use the designation 'VLA JHHMM.m+DDMM'. See also [SGL97] (GRB 970111), [FKN97b] (GRB 970508), [TFK98] (GRB 980329)
Ref:	=1997IAUC.6545Q...1F
by	FRAIL D.A. , KULKARNI S.R., NICASTRO L., DAL FIUME D., ORLANDINI M., PALAZZI E., PIZZICHINI G., FRONTERA F., ZAVATTINI G., AMATI L., CINTI M.N., COSTA E., FEROCI M., PIRO L., JAGER R., HEISE J., HURLEY K., KOUVELIOTOU C., FISHMAN G., MEEGAN C.
	IAU Circ., 6545, 1-None (1997)
	GRB 970111.
o	Radiosource named 'VLA J1528.7+1945' = <[FKN97] J1528.7+1945>, coincident with 'BeppoSAX source a'
o	<[FKN97] JHHMM.m+DDMM> N=1
Ref:	=1997ApJ...483L..91F
by	FRAIL D.A. , KULKARNI S.R., COSTA E., FRONTERA F., HEISE J., FEROCI M., PIRO L., DAL FIUME D., NICASTRO L., PALAZZI E., JAGER R.
	Astrophys. J., 483, 91-94 (1997)
	Radio monitoring of the 1997 January 11 γ-ray burst.
o	<[FKN97] JHHMM.m+DDMM> N=3 new sources added
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKN97a]
[FKN97a]	(Frail+Kulkarni+Nicastro+, 1997)
*****	Avoid the usage of [FKN97a], prefer [FKN97]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKN97b]
[FKN97b]	(Frail+Kulkarni+Nicastro+, 1997)= (VLA)
Write:	<<[FKN97b] JHHMM.m+DDMM>>
N:	1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=1 radio-source in the errorbox of GRB 970508. The authors use the designation 'VLA JHHMM.m+DDMM'. See also [FKN97] (GRB 970111), [SGL97] (GRB 970111), [TFK98] (GRB 980329)
Ref:	=1997Natur.389..261F
by	FRAIL D.A. , KULKARNI S.R., NICASTRO S.R., FEROCI M., TAYLOR G.B.
	Nature, 389, 261-263 (1997)
	The radio afterglow from the γ-ray burst of 8 May 1997.
o	VLA J065349.4+791619 = <[FKN97b] J0653.8+7916>
o	<[FKN97b] JHHMM.m+DDMM> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKO2012]
[FKO2012]	(Frail+Kulkarni+Ofek+, 2012)
Write:	<<[FKO2012] RT YYYYMMDD>>
N:	12 (SIMBAD class: Radio = Radio Source)
Note:	Re-analysis of archival data from the VLA for a sample of N=10 long-duration radio transients from 2007ApJ...666..346B.
Ref:	=2012ApJ...747...70F
by	FRAIL D.A. , KULKARNI S.R., OFEK E.O., BOWER G.C., NAKAR E.
	Astrophys. J., 747, 70 (2012)
	A revised view of the transient radio sky.
o	Table 1: <[FKO2012] RT YYYYMMDD> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKP2002]
[FKP2002]	(Fomalont+Kellermann+Partridge+, 2002)
Write:	<<[FKP2002] SA 13 NN>> <<[FKP2002] SA 13 a>> <<[FKP2002] Hercules NN>> <<[FKP2002] JHHMMSS+DDMMSS>> <<[FKP2002] mJy BHHMMSS+DDMMSS>> <<[FKP2002] mJy JHHMMSS+DDMMSS>>
N:	42+8+10+89
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Microjansky survey at 8.4GHz of 2 fields: SA 13 and Hercules fields defined by the authors. In SA 13 field, format 'NN' for 42 sources (see also [WFK95]), and format 'a' for 8 weaker radio-sources. Table 4: Catalog of N=89 microjansky sources at 8.4GHz (format mJy BHHMMSS+DDMMSS or mJy JHHMMSS+DDMMSS) in 5 fields defined in table 3.
Ref:	=2002AJ....123.2402F
by	FOMALONT E.B. , KELLERMANN K.I., PARTRIDGE R.B., WINDHORST R.A., RICHARDS E.A.
	Astron. J., 123, 2402-2416 (2002)
	The microjansky sky at 8.4 GHz.
o	(Erratum) erratum vol. 125, p. 2751 (2003)
o	Calibrator J1658+4749 is a misprint for QSO J1658+4737?
o	Table 1: <[FKP2002] SA 13 NN> (Nos 1-42) = <[FKP2002] JHHMMSS+DDMMSS> N=42, <[FKP2002] SA 13 a> (Nos a-h) = <[FKP2002] JHHMMSS+DDMMSS> N=8. Table 2: <[FKP2002] Hercules NN> (Nos 1-10) = <[FKP2002] JHHMMSS+DDMMSS> N=10. Table 4: <[FKP2002] mJy BHHMMSS+DDMMSS> N=6+14, <[FKP2002] mJy JHHMMSS+DDMMSS> N=29+34+6.
=E=	Catalogue in electronic form as J/AJ/123/2402
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKP2017]
[FKP2017]	(Fang+Kim+Pascucci+, 2017)
Write:	<<[FKP2017] NNN>>
N:	691
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	MMT Hectospec spectroscopic observations of N=691 young stars, centered on NGC 1980. Use of archival 2MASS, SDSS, UKIDSS, AAVSO data. See also [BAB2014].
in source:	NAME ORI A MCLD
in source:	NGC 1980
Ref:	=2017AJ....153..188F
by	FANG M. , KIM J.S., PASCUCCI I., APAI D., ZHANG L., SICILIA-AGUILAR A., ALONSO-MARTINEZ M., EIROA C., WANG H.
	Astron. J., 153, 188-188 (2017)
	NGC 1980 is not a foreground population of Orion: spectroscopic survey of young stars with low extinction in Orion A.
o	Table 6: <[FKP2017] NNN> (Nos 1-691).
=E=	Catalogue in electronic form as <J/AJ/153/188/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKR97]
[FKR97]	(Fomalont+Kellermann+Richards+, 1997)= (HDF) = (HFF)
Write:	<<[FKR97] MMSS+MMSS>>
N:	6+12
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Radio observations of the Hubble Deep Field and of Hubble Flanking Fields. In the format 'MMSS.s-MMSS', relative to 12h and +62deg, (2000 coordinates). Table 1: N=6 radio-sources in Hubble Deep Field. Table 2: N=12 radio-sources in Hubble Flanking Fields
in source:	NAME HDFN
Ref:	=1997ApJ...475L...5F
by	FOMALONT E.B. , KELLERMANN K.I., RICHARDS E.A., WINDHORST R.A., PATRIDGE R.B.
	Astrophys. J., 475, 5-8 (1997)
	Radio emission from objects in the Hubble Deep Field.
o	Format 'MMSS+MMSS' in 2000 coordinates, with 12h and +62° of RA and Dec
o	Tables 1, 2: <[FKR97] MMSS+MMSS> N=6+12
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKS2000]
[FKS2000]	(Frail+Kulkarni+Sari+, 2000)= (VLA)
Write:	<<[FKS2000] VLA JHHMMSS.s+DDMMSS>> <<[FKS2000] JHHMMSS.s+DDMM.m>>
N:	1+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=1 VLA radio-source, 'VLA J232221.5+771543', afterglow of GRB 980519, coincident with OT 19980519. N=1 field source, 2'5 from GRB 980519, 'J232137.6+7715.0'.
Ref:	=2000ApJ...534..559F
by	FRAIL D.A. , KULKARNI S.R., SARI R., TAYLOR G.B., SHEPHERD D.S., BLOOM J.S., YOUNG C.H., NICASTRO L., MASETTI N.
	Astrophys. J., 534, 559-564 (2000)
	The radio afterglow from GRB 980519: a test of the jet and circumstellar models.
o	<[FKS2000] VLA JHHMMSS.s+DDMMSS> N=1, <[FKS2000] JHHMMSS.s+DDMM.m> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKS2005]
[FKS2005]	(Falomo+Kotilainen+Scarpa+, 2005)
Write:	<<[FKS2005] 0045-3337 GN>> <<[FKS2005] 0101-337 GN>>
N:	1+2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ESO-VLT NIR adaptative optics images of 2 QSO: Near QSO 0045-3337, a companion galaxy is found, QSO 0101-337 is surrounded by a number of faint galaxies, the two closest ones are designated G1 and G2.
Ref:	=2005A&A...434..469F
by	FALOMO R. , KOTILAINEN J.K., SCARPA R., TREVES A.
	Astron. Astrophys., 434, 469-473 (2005)
	VLT adaptive optics imaging of QSO host galaxies and their close environment at z ~ 2.5: Results from a pilot program.
o	Fig.1: <[FKS2005] 0045-3337 GN> (No. G1), <[FKS2005] 0101-337 GN> (Nos G1-G2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKS2008]
[FKS2008]	(Furuya+Kitamura+Shinnaga, 2008)
Write:	<<[FKS2008] GF 9-NN>>
N:	10
Object:	NH3 MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	Nobeyama Radio Observatory 45m telescope observations of the NH3 lines in the GF 9 globular filament. See also [WCG99].
in source:	GF 9 = LDN 1082
Ref:	=2008PASJ...60..421F
by	FURUYA R.S. , KITAMURA Y., SHINNAGA H.
	PASJ, 60, 421-428 (2008)
	Low-mass star-forming cores in the GF9 filament.
o	Table 1: <[FKS2008] GF 9-NN> (Nos 9-1 to 9-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKS2019]
[FKS2019]	(Faramaz+Krist+Stapelfeldt+, 2019)
Write:	<<FKS2019 SN>>
N:	4
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 6 (230GHz, 1.3mm) observations of N=4 continuum sources in the field of HD 202628.
Ref:	=2019AJ....158..162F
by	FARAMAZ V. , KRIST J., STAPELFELDT K.R., BRYDEN G., MAMAJEK E.E., MATRA L., BOOTH M., FLAHERTY K., HALES A.S., HUGHES A.M., BAYO A., CASASSUS S., CUADRA J., OLOFSSON J., SU K.Y.L., WILNER D.J.
	Astron. J., 158, 162-162 (2019)
	From scattered-light to millimeter emission: a comprehensive view of the gigayear-old system of HD 202628 and its eccentric debris ring.
o	Fig. 2, Table 4: <[FKS2019] SN> (Nos S1-S4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKS99]
[FKS99]	(Furuya+Kitamura+Saito+, 1999) (Not yet in Simbad)
Write:	<<[FKS99] Red>> <<[FKS99] Blue>> <<[FKS99] Blue N>>
N:	2+3
Object:	H2O Maser component (SIMBAD class: Maser)
Note:	H2O maser components in 'NAME SH 2-106 FIR'. 'Red' for redshifted, 'Blue' for blueshifted.
in source:	SH 2-106:NAME SH 2-106 FIR = NAME SH 2-106 FIR
Ref:	=1999ApJ...525..821F
by	FURUYA R.S. , KITAMURA Y., SAITO M., KAWABE R., WOOTTEN H.A.
	Astrophys. J., 525, 821-831 (1999)
	VLA observations of H_{2}O masers in the class 0 protostar S106 FIR: evidence for a 10 AU scale accelerating jetlike flow.
o	Table 3: <[FKS99] Red>, <[FKS99] Blue>, <[FKS99] Blue N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FKSZ
FKSZ	(Russ.: General Catalog of Fundamental faint *)
Write:	<<FKSZ NNN>>
N:	587
Object:	Faint * (SIMBAD class: Star)
Ref:	=1958TrPul..72....5Z
by	ZVEREV M.S. , POLOZHENTSEV D.D.
	Tr. Glav. Astron. Obs. Pulkovo, ser. 2, 72, 5-76 (1958)
	A preliminary general catalogue of fundamental faint stars with declinations from +90° to -20 ° (FKSZ).
o	<FKSZ NNN> N=587 among (Nos 2-931)
=E=	Catalogue in electronic form as I/42
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [FKT2000]
[FKT2000]	(Flin+Krywult+Trevese+, 2000)
Write:	<<[FKT2000] ACO NNNN NNN>>
N:	1074
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
in source:	ACO 147
in source:	ACO 260
in source:	ACO 272
in source:	ACO 278
in source:	ACO 1661
in source:	ACO 2056
in source:	ACO 2073
in source:	ACO 2093
in source:	ACO 2096
in source:	ACO 2124
Ref:	=2000A&AS..146..373F
by	FLIN P. , KRYWULT J., TREVESE D., CIRIMELE G., HICKSON P.
	Astron. Astrophys., Suppl. Ser., 146, 373-375 (2000)
	Properties of nearby clusters of galaxies. IV. A147, A260, A272, A278, A1661, A2056, A2073, A2093, A2096, A2124.
o	Catalog: <[FKT2000] ACO NNNN NNN> N=1074.
=E=	Catalogue in electronic form as J/A+AS/146/373
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKT2001]
[FKT2001]	(Falomo+Kotilainen+Treves, 2001) (Not yet in Simbad)
Write:	<<[FKT2001] 0348-120 GN>> <<[FKT2001] 0402-362 HG>> <<[FKT2001] 0402-362 G>>
N:	3+2
Object:	G (SIMBAD class: Galaxy)
Note:	ESO VLT observations of QSO 0348-120 and QSO 0402-362 fields. N=3 galaxies near QSO 0348-120, (Nos G1-G3). N=1 Host galaxy (without designation in paper, 'HG' in SIMBAD) of QSO 0402-362, and N=1 companion galaxy (without designation in paper, 'G' in SIMBAD).
Ref:	=2001ApJ...547..124F
by	FALOMO R. , KOTILAINEN J., TREVES A.
	Astrophys. J., 547, 124-128 (2001)
	Near-infrared imaging of the host galaxies of three radio-loud quasars at z~1.5.
o	Figs 1: <[FKT2001] 0348-120 GN> (Nos G1-G3), <[FKT2001] 0402-362 HG> N=1, <[FKT2001] 0402-362 G> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKT2013]
[FKT2013]	(Fraga+Kunder+Tokovinin, 2013) (Not yet in Simbad)
Write:	<<[FKT2013] NNNN>>
N:	7416
Object:	* (SIMBAD class: Star)
Note:	SOAR SAM BVRI observations of N=7416 stars in the globular cluster NGC 6496.
in source:	NGC 6496
Ref:	=2013AJ....145..165F
by	FRAGA L. , KUNDER A., TOKOVININ A.
	Astron. J., 145, 165 (2013)
	SOAR adaptive optics observations of the globular cluster NGC 6496.
o	Table 2: <[FKT2013] NNNN> (Nos 1-7416).
o	In the abstract, NGC 6469 is a misprint for NGC 6496.
=E=	Catalogue in electronic form as <J/AJ/145/165/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKT92]
[FKT92]	(Fabbiano+Kim+Trinchieri, 1992)
Write:	<<[FKT92] NGC NNNN N>>
N:	19
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Einstein IPC and HRI observations. See also: [FT84], [FT87], [F88], [TFP88], [TFR90], TF
in source:	NGC 247
in source:	NGC 1313
in source:	NGC 3628
in source:	NGC 4236
in source:	NGC 2403
in source:	NGC 4258
in source:	NGC 4449
Ref:	=1992ApJS...80..531F
by	FABBIANO G. , KIM D.-W., TRINCHIERI G.
	Astrophys. J., Suppl. Ser., 80, 531-644 (1992)
	An X-ray catalog and atlas of galaxies.
o	Table 8A: <[FKT92] NGC NNNN N> N=3+2+2+2+4+2+4
=E=	Catalogue in electronic form as J/ApJS/80/531
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKT95]
[FKT95]	(Frogel+Kuchinski+Tiede, 1995)
Write:	<<[FKT95] NNN>>
N:	799
Object:	* in Cl* (SIMBAD class: Star)
in source:	Liller 1
Ref:	=1995AJ....109.1154F
by	FROGEL J.A. , KUCHINSKI L.E., TIEDE G.P.
	Astron. J., 109, 1154-1168 (1995)
	Infrared array photometry of metal rich globular clusters. II. Liller 1 - the most metal rich cluster?
o	Table 3: <[FKT95] NNN> (Nos 1-799)
=E=	Catalogue in electronic form as J/AJ/109/1154
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKV2013]
[FKV2013]	(Fang+Kim+van Boekel+, 2013)
Write:	<<[FKV2013] NNNN>>
N:	1388
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Note:	MMT Hectospec and MMT Hectochelle observations of N=1388 YSOs in LDN 1641. Use of UKIDSS, SDSS, 2MASS and WISE data. See also [FVW2009].
in source:	LDN 1641
Ref:	=2013ApJS..207....5F
by	FANG M. , KIM J.S., VAN BOEKEL R., SICILIA-AGUILAR A., HENNING T., FLAHERTY K.
	Astrophys. J., Suppl. Ser., 207, 5 (2013)
	Young stellar objects in Lynds 1641: disks, accretion, and star formation history.
o	Tables 2-6: <[FKV2013] NNNN> (Nos 1-1388).
=E=	Catalogue in electronic form as J/ApJS/207/5
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKW2005]
[FKW2005]	(Furuya+Kitamura+Wootten+, 2005) (Not yet in Simbad)
Write:	<<[FKW2005] IRAS 20050+2720 NN>>
N:	14
Object:	H2O Maser (SIMBAD class: Maser)
Note:	VLBA study of H2O masers toward IRAS 20050+2720.
in source:	IRAS 20050+2720
Ref:	=2005A&A...438..571F
by	FURUYA R.S. , KITAMURA Y., WOOTTEN A., CLAUSSEN M.J., KAWABE R.
	Astron. Astrophys., 438, 571-583 (2005)
	Proper motion of H_{2}O masers in IRAS 20050+2720 MMS1: an AU scale jet associated with an intermediate-mass class 0 source.
o	IRAS 20050+2720 MMS1 = [CRS97] IRAS 20050+2720 MMS 1
o	Fig.3: <[FKW2005] IRAS 20050+2720 NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKW2009]
[FKW2009]	(Fang+Kong+Wang, 2009)
Write:	<<[FKW2009] UDFNNNN>>
N:	24
Object:	Extremely Red Obj. (SIMBAD class: Galaxy)
Note:	N=24 EROs in the Hubble Ultra Deep Field. Use of HST (ACS and NICMOS) and Spitzer (MIPS), and VLT (ISAAC) data.
in source:	NAME HUDF
Ref:	=2009RAA.....9...59F
by	FANG G.-W. , KONG X., WANG M.
	RAA, 9, 59-72 (2009)
	Classification of extremely red objects in the Hubble Ultra Deep Field.
o	Figs 6-7, Table 1: <[FKW2009] UDFNNNN> N=24 among (Nos 15-1361).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FKW84]
[FKW84]	(Fomalont+Kellermann+Wall+, 1984)= (DSS) = ISS
Write:	<<[FKW84] DSS NN>> <<[FKW84] ISS NN>>
N:	16+35
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	N=16 and 35 sources respectively observed in the Deep Source Survey and the Intermediate Source Survey.
Ref:	=1984Sci...225...23F
by	FOMALONT E.B. , KELLERMANN K.I., WALL J.V., WEISTROP D.
	Science, 225, 23-28 (1984)
	A deep 6-centimeter radio source survey.
o	Table 3: <[FKW84] DSS NN> (Nos 1-16). Table 4: <[FKW84] ISS NN> (Nos 1-35) = <ISS NN> (Nos 1-35).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Fl
Fl	(Florsch)
*****	Avoid the usage of Fl, prefer Flo
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Fl
Fl	(Fleming)
*****	Avoid the usage of Fl, prefer Fg
Details on Acronym: FL
FL	(Finding List)
*****	Avoid the usage of FL, prefer [WOF80]
Origin	of the Acronym: L (1998IBVS.4601....1W,1998IBVS.4605....1S)
Details on Acronym: [FL2002]
[FL2002]	(Fassnacht+Lubin, 2002)
Write:	<<[FL2002] GrG>> <<[FL2002] +NNN+NNN>>
N:	1+34+12
Object:	Group of G + G (SIMBAD class: Galaxy)
Note:	Keck LRIS observations of the region of CLASS B0712+472. N=1 group of galaxies at z=0.2909 coincident with CLASS B0712+472. N=46 galaxies in the field of the CLASS lensing system. In the format the 2 parts are the distance in RA (in arcsecond) and in Dec (in arcsecond) from the lensing galaxy [JNB98] B0712+472 G.
Ref:	=2002AJ....123..627F
by	FASSNACHT C.D. , LUBIN L.M.
	Astron. J., 123, 627-636 (2002)
	The gravitational lens-galaxy group connection. I. Discovery of a group coincident with CLASS B0712+472.
o	Text: <[FL2002] GrG> N=1. Tables 1, 2: <[FL2002] +NNN+NNN> N=34+12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FL2004]
[FL2004]	(Feilgelson+Lawson, 2004)
Write:	<<[FL2004] NNN>>
N:	107
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of PMS stars in Cha I North Cloud. See also CHXR
in source:	NAME Cha I
Ref:	=2004ApJ...614..267F
by	FEIGELSON E.D. , LAWSON W.A.
	Astrophys. J., 614, 267-283 (2004)
	An X-ray census of young stars in the Chamaeleon I North cloud.
o	Table 1: <[FL2004] NNN> (Nos 1-107).
=E=	Catalogue in electronic form as J/ApJ/614/267
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FL29
FL29	(Field No. FL29)
Write:	<<FL29 A>>
N:	9
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Table 3: (Nos A-H) and p. 267: No. X
Ref:	=1995AJ....110..259G
by	GREGORICH D.T. , NEUGEBAUER G., SOIFER B.T., GUNN J.E., HERTER T.L.
	Astron. J., 110, 259-267 (1995)
	Study of deep IRAS fields at 60 microm.
o	Table 3: <FL29 A> (Nos A-H) and p. 267: No. X
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FL8Y
FL8Y	(Fermi-LAT 8-year Source List)
Write:	<<FL8Y JHHMM.m+DDMM>> <<FL8Y JHHMM.m+DDMM{e\|i}>>
N:	5523
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	Preliminary Fermi LAT list of N=5523 sources above 4σ significance, based on the first eight years of science data from the Fermi Gamma-ray Space Telescope mission and the 100MeV-1TeV range.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FLAMINGOS
FLAMINGOS	(Florida Multi-Object Imaging Near-Infrared Grism Observational Spectrometer)
*****	Avoid the usage of FLAMINGOS, prefer [WFT2009]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FLAMINGOS
FLAMINGOS	(Florida Multi-Object Imaging Near-Infrared Grism Observational Spectrometer)
*****	Avoid the usage of FLAMINGOS, prefer [WFT2010]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FLAMINGOS
FLAMINGOS	(Florida Multi-Object Imaging Near-Infrared Grism Observational Spectrometer)
*****	Avoid the usage of FLAMINGOS, prefer [WTF2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FLASH
FLASH	(FLAIR Shapley-Hydra survey)
Write:	<<FLASH JHHMMSS.ss+DDMMSS.s>>
N:	4613
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	The catalog consists of 4613 galaxies brigter than b(J) 16.7 over a region of the sky in the general direction of the Local Group motion.
Ref:	=2003MNRAS.339..652K
by	KALDARE R. , COLLESS M., RAYCHAUDHURY S., PETERSON B.A.
	Mon. Not. R. Astron. Soc., 339, 652-662 (2003)
	FLASH redshift survey - I. Observations and catalogue.
o	In the catalog, coordinates are J2000 coordinates.
o	Catalog: <FLASH JHHMMSS.ss+DDMMSS.s> N=4613.
=E=	Catalogue in electronic form as J/MNRAS/339/652
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FLB2020]
[FLB2020]	(Fuller+Lemaux+Bradac+, 2020)
Write:	<<[FLB2020] ANNNN.NNN>> <<[FLB2020] MACSHHMM.NN>> <<[FLB2020] RXJ1347.NN>> <<[FLB2020] NNNN.NNN>> (not recognised by Simbad, but found in literature)
N:	4+24+8
Object:	Lyman alpha emitting G (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck DEIMOS observations of N=36 Ly alpha emitting galaxies in the fields of ten galaxy clusters. Use of CLASH, SURFSUP, GLASS, ASTRODEEP data.
Ref:	=2020ApJ...896..156F
by	FULLER S. , LEMAUX B.C., BRADAC M., HOAG A., SCHMIDT K.B., HUANG K., STRAIT V., MASON C., TREU T., PENTERICCI L., TRENTI M., HENRY A., MALKAN M.
	Astrophys. J., 896, 156-156 (2020)
	Spectroscopically confirmed Lyα emitters from redshift 5 to 7 behind 10 galaxy cluster lenses.
o	Fig. B1, Table B1: <[FLB2020] ANNN.NNN> N=4, <[FLB2020] MACSHHMM.NN> N=24, <[FLB2020] RXJ1347.NN> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLC2006]
[FLC2006]	(Floyd+Lang+Chaberge+, 2006)= ([FLC2006a]) (Not yet in Simbad)
Write:	<<[FLC2006] AN>>
N:	4+3+2
Object:	(Rad) + G (SIMBAD class: Radio = Radio Source)
Note:	HST NICMOS observations of 3C 133: N=3 radio features in the jet (Nos A-D), N=3 radio jet knots (Nos E1-E3), and N=2 nearby galaxies (Nos G1-G2).
in source:	3C 133
Ref:	=2006ApJ...643..660F
by	FLOYD D.J.E. , LAING R., CHIABERGE M., PERLMAN E., SPARKS W., MACCHETTO D., MADRID J., AXON D., O'DEA C.P., BAUM S., QUILLEN A., MILEY G., CAPETTI A.
	Astrophys. J., 643, 660-666 (2006)
	An optical-infrared jet in 3C 133.
o	Fig.1: <[FLC2006] AN> (Nos A-D, E1-E3, G1-G2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLC2006a]
[FLC2006a]	(Floyd+Lang+Chaberge+, 2006) (Not yet in Simbad)
*****	Avoid the usage of [FLC2006a], prefer [FLC2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLC2006b]
[FLC2006b]	(Fynbo+Limousin+Castro Ceron+, 2006)
Write:	<<[FLC2006b] GRB 060206 abs N.NNN>>
N:	1
Object:	Absorber
Note:	Spectroscopic observations of GRB 060206. See also [FSL2006] and [HSD2007].
Ref:	=2006GCN..4692....1F
by	FYNBO J.P.U. , LIMOUSIN M., CASTRO CERON J.M., JENSEN B.L., NARANEN J.
	GRB Coordinates Network, Circular Service, 4692, 1-None (2006)
	GRB 060206: spectroscopic redshift.
o	<[FLC2006b] GRB 060206 abs N.NNN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLC2013]
[FLC2013]	(Frebel+Lunnan+Casey+, 2013)
Write:	<<[FLC2013] 300S-NN>>
N:	52
Object:	* (SIMBAD class: Star)
Note:	Magellan Clay telescope MIKE spectroscopy. Sample of N=52 stars, candidate members of a 300km/s stream, a stream independent of Segue 1.
in source:	NAME Segue 1 Stream
Ref:	=2013ApJ...771...39F
by	FREBEL A. , LUNNAN R., CASEY A.R., NORRIS J.E., WYSE R.F.G., GILMORE G.
	Astrophys. J., 771, 39 (2013)
	The 300 km/s stellar stream near Segue 1: insights from high-resolution spectroscopy of its brightest star.
o	Table 1: <[FLC2013] 300S-NN> (Nos 1-52).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLC2020]
[FLC2020]	(Feng+Li+Caselli+, 2020)
Write:	<<[FLC2020] GLLL.ll+BB.bb PN>> <<[FLC2020] GLL.ll+B.bb PN>> (not recognised by Simbad, but found in literature)
N:	12
Object:	Core (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	IRAM 30 m and NRO 45 m telescopes observations of N=12 peaks in the field of four regions, as part of the Multiwavelength line-Imaging survey of the 70µm-dArk and bright clOuds (MIAO).
Ref:	=2020ApJ...901..145F
by	FENG S. , LI D., CASELLI P., DU F., LIN Y., SIPILA O., BEUTHER H., SANHUEZA P., TATEMATSU K., LIU S.Y., ZHANG Q., WANG Y., HOGGE T., JIMENEZ-SERRA I., LU X., LIU T., WANG K., ZHANG Z.Y., ZAHORECZ S., LI G., LIU H.B., YUAN J.
	Astrophys. J., 901, 145-145 (2020)
	The chemical structure of young high-mass star-forming clumps. II. Parsec-scale CO depletion and deuterium fraction of HCO^+.
o	Fig. 1, Table 2: <[FLC2020] GLLL.ll+BB.bb PN> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLD2014]
[FLD2014]	(Fiorentino+Lanzoni+Dalessandro+, 2014)
Write:	<<[FLD2014] WUMa N>> <<[FLD2014] SXP N>>
N:	12
Object:	WU* + SX* (SIMBAD class: BlueStraggler = Blue Straggler)
Stat:	is completely incorporated in Simbad
Note:	HST WFC3 observations of N=9+3 variable blue straggler stars in the central region of the Galactic globular cluster NGC 6541.
in source:	NGC 6541
Ref:	=2014ApJ...783...34F
by	FIORENTINO G. , LANZONI B., DALESSANDRO E., FERRARO F.R., BONO G., MARCONI M.
	Astrophys. J., 783, 34 (2014)
	Blue straggler masses from pulsation properties. I. The case of NGC 6541.
o	Table 1: <[FLD2014] WUMa N> (Nos 1-3) = <Cl* NGC 6541 SAW VNN> (Nos V9-V11), <[FLD2014] SXP N> (Nos 1-9) = <Cl* NGC 6541 SAW VNN> (Nos V12-V20).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 1FLE
1FLE	(First Fermi/LAT Low Energy catalog)
Write:	<<1FLE JHHMM+DDMM>>
N:	198
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	The first Fermi Large Area Telescope (LAT) low energy catalog (1FLE) contains N=198 sources detected above 3σ significance in the energy range 30-100MeV. Use of eight years and nine months of Fermi LAT data.br More information can be found at https://fermi.gsfc.nasa.gov/
Ref:	=2018A&A...618A..22P
by	PRINCIPE G. , MALYSHEV D., BALLET J., FUNK S.
	Astron. Astrophys., 618A, 22-22 (2018)
	The first catalog of Fermi-LAT sources below 100 MeV.
o	<1FLE JHHMM+DDMM> N=198.
=E=	Catalogue in electronic form as <J/A+A/618/A22/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Fleming
Fleming	(Fleming)
*****	Avoid the usage of Fleming, prefer Fg
Details on Acronym: FLEX
FLEX	(FLEX system)
*****	Avoid the usage of FLEX, prefer [LGC91]
Origin	of the Acronym: L (1997MNRAS.287..899L)
Details on Acronym: [FLF2000]
[FLF2000]	(Fox+Lewin+Fabian+, 2000) (Not yet in Simbad)
Write:	<<[FLF2000] A>>
N:	6
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT and ASCA sources mear SN 1995N.
Ref:	=2000MNRAS.319.1154F
by	FOX D.W. , LEWIN W.H.G., FABIAN A., IWASAWA K., TERLEVICH R., ZIMMERMANN H.U., ASCHENBACH B., WEILER K., VAN DYK S., CHEVALIER R., RUTLEDGE R., INOUE H., UNO S.
	Mon. Not. R. Astron. Soc., 319, 1154-1158 (2000)
	The X-ray spectrum and light curve of Supernova 1995N.
o	Fig.1: <[FLF2000] A> (Nos A-F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLF2016]
[FLF2016]	(Faesi+Lada+Forbrich, 2016)
Write:	<<[FLF2016] DCLNNNA-N>>
N:	45
Object:	Giant MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	SMA CO observations of N=45 giant molecular clouds (GMCs) in 11 star-forming regions in the spiral galaxy NGC 300.
in source:	NGC 300
Ref:	=2016ApJ...821..125F
by	FAESI C.M. , LADA C.J., FORBRICH J.
	Astrophys. J., 821, 125-125 (2016)
	Resolving giant molecular clouds in NGC 300: a first look with the submillimeter array.
o	Table 3: <[FLF2016] DCLNNNA-N> N=45 among (Nos DCL23-1 to DCL137-6).
=E=	Catalogue in electronic form as J/ApJ/821/125
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLF2018]
[FLF2018]	(Faesi+Lada+Forbrich, 2018)
Write:	<<[FLF2018] DCLNNNA-ANN>>
N:	299
Object:	Giant MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 6 12CO(2-1) observations of N=299 giant molecular clouds (GMCs) in NGC 300 close to 48 HII regions from the Deharveng et al. (1988A&AS...73..407D, see [DCL88]) catalog. See also [FLF2016], for a pilot study with SMA, in a sub-sample of 10 HII regions.
in source:	NGC 300
Ref:	=2018ApJ...857...19F
by	FAESI C.M. , LADA C.J., FORBRICH J.
	Astrophys. J., 857, 19-19 (2018)
	The ALMA view of GMCs in NGC 300: physical properties and scaling relations at 10 pc resolution.
o	Table 7: <[FLF2018] DCLNNNA-ANN> N=299.
=E=	Catalogue in electronic form as <J/ApJ/857/19/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLG2003]
[FLG2003]	(Feigelson+Lawson+Garmire, 2003)= (eps Cha)
Write:	<<[FLG2003] eps Cha NN>> <<[FLG2003] JHHMMSS.s+DDMMSS.s>>
N:	21+10+19
Object:	*inCl + (X) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of the eps Cha Group of stars. N=21 stars are members of the group. N=10 new X-ray selected members of the 'OSCA' association (Oph-Sco-Cen Assoc.).
in source:	NAME EPS CHA GROUP
Ref:	=2003ApJ...599.1207F
by	FEIGELSON E.D. , LAWSON W.A., GARMIRE G.P.
	Astrophys. J., 599, 1207-1222 (2003)
	The ε Chamaeleontis young stellar group and the characterization of sparse stellar clusters.
o	(Erratum) erratum vol.649, p. 1184 (2006)
o	Table 3: <[FLG2003] eps Cha N> (Nos 1-9). Table 4: <[FLG2003] JHHMMSS.s+DDMMSS.s> N=10.
Ref:	=2004ApJ...616.1033L
by	LUHMAN K.L.
	Astrophys. J., 616, 1033-1041 (2004)
	A survey for low-mass stars and brown dwarfs in the η Chamaeleontis and ε Chamaeleontis young associations.
o	Table 3: <[FLG2003] eps Cha NN> (Nos 10-12) added.
Ref:	=2008ApJ...675.1375L
by	LUHMAN K.L. , ALLEN L.E., ALLEN P.R., GUTERMUTH R.A., HARTMANN L., MAMAJEK E.E., MEGEATH S.T., MYERS P.C., FAZIO G.G.
	Astrophys. J., 675, 1375-1406 (2008)
	The disk population of the Chamaeleon I star-forming region.
o	Tables 4-7: <[L2007b] Cha JHHMMSSss+DDMMSSs> N=17 added. Table 11: <[FLG2003] eps Cha NN> (Nos 13-21) added.
Ref:	=2013MNRAS.435.1325M
by	MURPHY S.J. , LAWSON W.A., BESSELL M.S.
	Mon. Not. R. Astron. Soc., 435, 1325-1349 (2013)
	Re-examining the membership and origin of the ε Cha association.
o	Table 7: <[FLG2003] eps Cha NN> (Nos 22-40) added.
=E=	Catalogue in electronic form as J/ApJ/675/1375
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLG99]
[FLG99]	(Fiore+La Franca+Giommi+, 1999)
Write:	<<[FLG99] JHHMM.m+DDMMA>>
N:	2
Object:	Opt. Candidate (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=2 possible optical candidates (Blue broad-line QSOs) of the HELLAS source SAX J1118.8+4026. See also HELLAS.
Ref:	=1999MNRAS.306L..55F
by	FIORE F. , LA FRANCA F., GIOMMI P., ELVIS M., MATT G., COMASTRI A., MOLENDI S., GIOIA I.
	Mon. Not. R. Astron. Soc., 306, 55-60 (1999)
	The contribution of faint active galactic nuclei to the hard X-ray background.
o	Table 1: <[FLG99] JHHMM.m+DDMMA> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLH2020]
[FLH2020]	(Fahrion+Lyubenova+Hilker+, 2020)
Write:	<<[FLH2020] JDDD.ddddddd+DD.ddddddd>>
N:	722
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Note:	VLT MUSE observations of N=722 globular clusters in the inner regions of 32 galaxies in the Fornax cluster, as part of the Fornax 3D project.
in source:	NAME Fornax Cluster
Ref:	=2020A&A...637A..26F
by	FAHRION K. , LYUBENOVA M., HILKER M., VAN DE VEN G., FALCON-BARROSO J., LEAMAN R., MARTIN-NAVARRO I., BITTNER A., COCCATO L., CORSINI E.M., GADOTTI D.A., IODICE E., McDERMID R.M., PINNA F., SARZI M., VIAENE S., DE ZEEUW P.T., ZHU L.
	Astron. Astrophys., 637A, 26-26 (2020)
	The Fornax 3D project: Globular clusters tracing kinematics and metallicities.
o	gc-cat.dat: <[FLH2020] JDDD.ddddddd+DD.ddddddd> N=722.
=E=	Catalogue in electronic form as <J/A+A/637/A26/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLH92]
[FLH92]	(Fort+Le Fevre+Hammer+, 1992)
Write:	<<[FLH92] GNN>> <<[FLH92] GNN'>> <<[FLH92] ANN>> <<[FLH92] ANN SKN>> <<[FLH92] AR>> <<[FLH92] ARN>>
N:	32+1+11+3+4
Object:	G + Arc (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	(Nos G1-G32) Galaxies in the lensing cluster MS 2137-23 = 1E 2137.3-2353 (Nos A0-A10) for Arcs (sources of these arcs are [HGS97] S1 to S3 sources). Giant tangential arc A0 is broken in 3 segments A01, A02, A03. AO1 and A02 are subdivided in 2 'subknots' SK1 and SK2. 'AR' and 'ARN' are 2 radial arcs (ARN North of AR).
in source:	1E 2137.0-2353
Ref:	=1992ApJ...399L.125F
by	FORT B. , LE FEVRE O., HAMMER F., CAILLOUX M.
	Astrophys. J., 399, 125-127 (1992)
	An arc system with a radial gravitational image in the cluster MS 2137-23.
o	Table 1: Table 1: <[FLH92] GNN> (Nos G1-G32), <[FLH92] ANN> (Nos A0, A01, A02, A1-A10)
Ref:	=1993ApJ...407...33M
by	MELLIER Y. , FORT B., KNEIB J.-P.
	Astrophys. J., 407, 33-45 (1993)
	The dark matter distribution in MS 2137-23 from the modeling of the multiple arc systems.
o	MS 2137-23 = 1E 2137.3-2353, Radial Arc later designated as [FLH92] AR.
o	Fig.4: <[FLH92] A03> N=1 added, <[FLH92] GNN'> (No. G29') added.
Ref:	=1997ApJ...491..477H
by	HAMMER F. , GIOIA I.M., SHAYA E.J., TEYSSANDIER P., LE FEVRE O., LUPPINO G.A.
	Astrophys. J., 491, 477-482 (1997)
	Detailed lensing properties of the MS 2137-2353 core and reconstruction of sources from Hubble Space Telescope imagery.
o	Fig.2: <[FLH92] AR> N=1 added, <[FLH92] ARN> N=1 added, <[FLH92] A01 SKN> (Nos SK1-SK2) added, <[FLH92] A02 SKN> (Nos SK1-SK2) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLH96]
[FLH96]	(Fuller+Ladd+Hodapp, 1996)
Write:	<<[FLH96] LDN 1527 A>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
in source:	LDN 1527
Ref:	=1996ApJ...463L..97F
by	FULLER G.A. , LADD E.F., HODAPP K.-W.
	Astrophys. J., 463, 97-100 (1996)
	Lynds 1527: an embedded protobinary system in Taurus.
o	p. L100 : IRAS 16293 = IRAS 16293-2422
o	Table 2: <[FLH96] LDN 1527 A> (Nos A-B)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLM2007]
[FLM2007]	(Fingerhut+Lee+McCall+, 2007)
Write:	<<[FLM2007] Maffei 2 (+xxxx+yyyy)>> <<[FLM2007] IC 342 (+xxxx+yyyy)>> <<[FLM2007] NGC NNNN (+xxxx+yyyy)>>
N:	2+6+73
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	KPNO Mayall 4m telescope observations of Maffei 2 and IC 342. HII regions in 12 galaxies. In the format '+xxxx+yyyy' stands for offset in seconds from the center of the galaxy,
Ref:	=2007ApJ...655..814F
by	FINGERHUT R.L. , LEE H., McCALL M.L., RICHER M.G.
	Astrophys. J., 655, 814-830 (2007)
	The extinction and distance of Maffei 2 and a new view of the IC 342/Maffei group.
o	Table 2: <[FLM2007] Maffei 2 (+xxxx+yyyy)> N=2, <[FLM2007] IC 342 (+xxxx+yyyy)> N=6. Table 4: <[FLM2007] NGC NNNN (+xxxx+yyyy)> N=73.
=E=	Catalogue in electronic form as J/ApJ/655/814
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLM2008]
[FLM2008]	(Forbrich+Lada+Muench+, 2008)
Write:	<<[FLM2008] NN>>
N:	26
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Spitzer MIPS image of NGC 2547.
in source:	NGC 2547
Ref:	=2008ApJ...687.1107F
by	FORBRICH J. , LADA C.J., MUENCH A.A., TEIXEIRA P.S.
	Astrophys. J., 687, 1107-1116 (2008)
	New M dwarf debris disk candidates in NGC 2547.
o	Table 2: <[FLM2008] NN> (Nos 1-26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLM2009]
[FLM2009]	(Forbrich+Lada+Muench+, 2009)
Write:	<<[FLM2009] NN>>
N:	26
Object:	Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Stat:	is completely incorporated in Simbad
Note:	Spitzer MIPS and IRAC observations of the Pipe Nebula.
in source:	NAME PIPE Nebula
Ref:	=2009ApJ...704..292F
by	FORBRICH J. , LADA C.J., MUENCH A.A., ALVES J., LOMBARDI M.
	Astrophys. J., 704, 292-305 (2009)
	A Spitzer census of star formation activity in the Pipe Nebula.
o	Tables 1-2: <[FLM2009] NN> (Nos 1-26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLM2010]
[FLM2010]	(Ford+Lockman+Mcclure-Griffiths, 2010) (Not yet in Simbad)
Write:	<<[FLM2010] GLLL.ll+BB.bb>>
N:	255
Object:	HI Cloud (SIMBAD class: HI = HI (21cm) Source)
Note:	N=255 HI clouds in the lower Galactic halo. Use of data from the Parkes Radio Telescope's Galactic All Sky Survey (GASS).
Ref:	=2010ApJ...722..367F
by	FORD H.A. , LOCKMAN F.J., McCLURE-GRIFFITHS N.M.
	Astrophys. J., 722, 367-379 (2010)
	Milky Way disk-halo transition in H I: properties of the cloud population.
o	Tables 1-2: <[FLM2010] GLLL.ll+BB.bb> N=255.
=E=	Catalogue in electronic form as J/ApJ/722/367
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLM96]
[FLM96]	(Fox+Lewin+Margon+, 1996)
Write:	<<[FLM96] M 92 A>> <<[FLM96] M 13 A>> <<[FLM96] M 13 Aa>> <<[FLM96] M 13 A-WW>>
N:	7+19+1+6
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT HRI observations. X-ray sources in M 92, N=7 sources (Nos A-G). X-ray sources in M 13, N=16 sources among (Nos A-T), another source has been added later: 'M 13 G-SE', and source 'G' divided in 2 components 'Ga' and 'Gb'.
in source:	M 92 = NGC 6341
in source:	M 13 = NGC 6205
Ref:	=1996MNRAS.282.1027F
by	FOX D. , LEWIN W., MARGON B., VAN PARADIJS J., VERBUNT F.
	Mon. Not. R. Astron. Soc., 282, 1027-1032 (1996)
	ROSAT HRI observations of the globular clusters M 13 and M 92.
o	Table 1: <[FLM96] M 92 A> (Nos A-G). Table 2: <[FLM96] M 13 A> N=12 among (Nos A-Q)
Ref:	=1997MNRAS.292L..45F
by	FERRARO F.R. , PALTRINIERI B., FUSI PECCI F., ROOD R.T., DORMAN B.
	Mon. Not. R. Astron. Soc., 292, 45-49 (1997)
	Faint ultraviolet objects in the core of M13: optical counterparts of the low-luminosity X-ray source?
o	Table 2: <[FLM96] M 13 G-SE> is new. Table 2: <Cl* NGC 6205 FPF NNNNN> N=3 stars from authors' list
Ref:	=2001A&A...368..137V
by	VERBUNT F.
	Astron. Astrophys., 368, 137-159 (2001)
	A census with ROSAT of low-luminosity X-ray sources in globular clusters.
o	Table 2: see also [FLM96], [HCJ97], [HG83b], [HGB93], [JVH94], [JVH96], [RDL94].
o	Table 2: <[V2001] NGC NNNN XNNa> N=49, <[V2001] JHHMMSS.ss+DDMMSS.s> N=2, <[FLM96] M 13 Aa> (Nos F, Ga-Gb, R-T) added, <[HCJ97] NN> (Nos 6-10) added, <[HGB93] A> (No. G) added, <[JVH94] NGC 6626 NNa> (Nos 5-12, 2a-2c) added, <[JVH94] NGC 6656 N> (No. 9) added, <[JVH94] NGC 7099 NN> (No. 13) added, <[JVH96] NGC 6121 NN> (Nos 7-10) added, <[JVH96] NGC 6352 NN> (No. 17) added, <[JVH96] NGC 6366 NN> (Nos 7-8) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLM99]
[FLM99]	(Filippenko+Leonard+Matheson+, 1999)
Write:	<<[FLM99] Star A>>
N:	6
Object:	* (SIMBAD class: Star)
Note:	Stars in the field of Nova Vel 1993. See also [SVC96], [DBC97].
Ref:	=1999PASP..111..969F
by	FILIPPENKO A.V. , LEONARD D.C., MATHESON T., LI W., MORAN E.C., RIESS A.G.
	Publ. Astron. Soc. Pac., 111, 969-979 (1999)
	A black hole in the X-ray Nova Velorum 1993.
o	Fig.1: <[DBC97] Star A> (Nos B-C) added. Fig.9: <[FLM99] Star A> (Nos A-F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FLMN
FLMN	(FLAMINGOS survey)
Write:	<<FLMN JHHMMSSs+DDMMSSs>>
N:	71
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	KPNO 2.1m and 4m telescopes FLAMINGOS observations to search for stars in NGC 2024. See also Cl* NGC 2024 LSE.
in source:	NGC 2024
Ref:	=2006ApJ...646.1215L
by	LEVINE J.L. , STEINHAUER A., ELSTON R.J., LADA E.A.
	Astrophys. J., 646, 1215-1229 (2006)
	Low-mass stars and brown dwarfs in NGC 2024: constraints on the substellar mass function.
o	Table 3, col(1): <Cl* NGC 2024 LSE NN> (Nos 1-71) = Table 3, col(2): <FLMN JHHMMSSs+DDMMSSs> N=71.
=E=	Catalogue in electronic form as J/ApJ/646/1215
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLN2011]
[FLN2011]	(Fynbo+Ledoux+Noterdaeme+, 2011) (Not yet in Simbad)
Write:	<<[FLN2011] QSO J0918+1636 abs 2.5832>> <<[FLN2011] Q0918+1636 abs 2.5832>> (not recognised by Simbad, but found in literature)
N:	1
Object:	G (SIMBAD class: Galaxy)
Note:	VLT X-shooter observations of the galaxy counterpart of a DLA on the line of site to the QSO J0918+1636.
Ref:	=2011MNRAS.413.2481F
by	FYNBO J.P.U. , LEDOUX C., NOTERDAEME P., CHRISTENSEN L., MOELLER P., DURGAPAL A.K., GOLDONI P., KAPER L., KROGAGER J.-K., LAURSEN P., MAUND J.R., MILVANG-JENSEN B., OKOSHI K., RASMUSSEN P.K., THORSEN T.J., TOFT S., ZAFAR T.
	Mon. Not. R. Astron. Soc., 413, 2481-2488 (2011)
	Galaxy counterparts of metal-rich damped Lyα absorbers – II. A solar-metallicity and dusty DLA at z_{abs}= 2.58.
o	<[FLN2011] QSO J0918+1636 abs 2.5832> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLN2017]
[FLN2017]	(Falocco+Larsson+Nandi, 2017)
Write:	<<[FLN2017] NGC 6217 knotN>>
N:	3
Object:	Knot (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of N=3 X-ray knots in a possible jet of the galaxy NGC 6217. Use of ROSAT, HST, and VLA archival observations.
in source:	NGC 6217
Ref:	=2017MNRAS.472.2280F
by	FALOCCO S. , LARSSON J., NANDI S.
	Mon. Not. R. Astron. Soc., 472, 2280-2288 (2017)
	A (likely) X-ray jet from NGC6217 observed by XMM-Newton.
o	Table 2: <[FLN2017] NGC 6217 knotN> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Flo
Flo	(Florsch)= (Fl)
Write:	<<Flo NNN>>
N:	776
Object:	* (SIMBAD class: Star)
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1972POStr...2....1F
by	FLORSCH A.
	Publ. Obs. Strasbourg, 2, 1-129 (1972)
	Etude du Petit Nuage de Magellan par la technique du prisme-objectif de Fehrenbach.
o	Tables I to IV: <Flo NNN> (Nos 1-776)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [FLR2004]
[FLR2004]	(Fadda+Lari+Rodighiero+, 2004)
Write:	<<[FLR2004] JHHMMSS.sss+DDMMSS.ss>>
N:	21
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Calibration stars in the ISO-LHSS survey.
Ref:	=2004A&A...427...23F
by	FADDA D. , LARI C., RODIGHIERO G., FRANCESCHINI A., ELBAZ D., CESARSKY C., PEREZ-FOURNON I.
	Astron. Astrophys., 427, 23-34 (2004)
	ISOCAM observations in the Lockman Hole. I. The 14.3 µm shallow survey: Data reduction, catalogue, and optical identifications.
o	Unusual truncation of ISO-LHSS: JHHMMSS+DDMMS
o	Table 2: <[FLR2004] JHHMMSS.sss+DDMMSS.ss> N=21. Tables 3, 4: <ISO-LHSS JHHMMSS+DDMMS> N=259+197.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLR2014]
[FLR2014]	(Foster+Lux+Romanowsky+, 2014)
Write:	<<[FLR2014] {p}{1\|2} {sup} NNN>> <<[FLR2014] p1 PN NN>> <<[FLR2014] p1 HST N>> <<[FLR2014] p2 HII NN>> <<[FLR2014] NGC4651 nuc>>
N:	913+1
Object:	Gl? + HII + Poss. PN (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Subaru Suprime-Cam and Keck DEIMOS observations of N=913+46 globular clusters candidates, planetary nebulae candidates, HII regions candidates to study the Umbrella Galaxy: NGC 4651.
in source:	NGC 4651
Ref:	=2014MNRAS.442.3544F
by	FOSTER C. , LUX H., ROMANOWSKY A.J., MARTINEZ-DELGADO D., ZIBETTI S., ARNOLD J.A., BRODIE J.P., CIARDULLO R., GABANY R.J., MERRIFIELD M.R., SINGH N., STRADER J.
	Mon. Not. R. Astron. Soc., 442, 3544-3564 (2014)
	Kinematics and simulations of the stellar stream in the halo of the Umbrella Galaxy.
o	Tables 2-5: <[FLR2014] p1 HST N> N=4 (Nos 0-3), <[FLR2014] p1 PN NN> N=39 (Nos 0-38), <[FLR2014] p1 sup NNN> N=251 (Nos 0-250), <[FLR2014] p2 sup NNN> N=557 (Nos 0-556), <[FLR2014] p2 HII NN> N=64 (Nos 0-63), <[FLR2014] NGC4651 nuc>.
=E=	Catalogue in electronic form as J/MNRAS/442/3544
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FLS
FLS	(First Look Survey)
*****	Avoid the usage of FLS, prefer [MWL2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FLS
FLS	(First Look Survey)
*****	Avoid the usage of FLS, prefer [SW2005]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FLS-R
FLS-R	(First-Look Survey, R-band)
Write:	<<FLS-R JHHMMSS.s+DDMMSS>>
N:	1226150
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	R band observations of Spitzer First Look Survey (FLS) and ELAIS fields at the 4m Mayall telescope at KPNO.
Ref:	=2004AJ....128....1F
by	FADDA D. , JANNUZI B.T., FORD A., STORRIE-LOMBARDI L.J.
	Astron. J., 128, 1-15 (2004)
	The Spitzer Space Telescope first-look survey: KPNO Mosaic-1 R-band images and source catalogs.
o	Catalogues: <FLS-R JHHMMSS.s+DDMMSS> N=1226150.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FLS160
FLS160	(First Look Survey, 160mu.m)
Write:	<<FLS160 JHHMMSS.s+DDMMSS>>
N:	227
Object:	(submm) (SIMBAD class: Infrared = Infra-Red Source)
Note:	160 mu.m observations from the Spitzer extragalactic First Look Survey.
Ref:	=2006AJ....131..250F
by	FRAYER D.T. , FADDA D., YAN L., MARLEAU F.R., CHOI P.I., HELOU G., SOIFER B.T., APPLETON P.N., ARMUS L., BECK R., DOLE H., ENGELBRACHT C.W., FANG F., GORDON K.D., HEINRICHSEN I., HENDERSON D., HESSELROTH T., IM M., KELLY D.M., LACY M., LAINE S., LATTER W.B., MAHONEY W., MAKOVOZ D., MASCI F.J., MORRISON J.E., MOSHIR M., NORIEGA-CRESPO A., PADGETT D.L., PESENSON M., SHUPE D.L., SQUIRES G.K., STORRIE-LOMBARDI L.J., SURACE J.A., TEPLITZ H.I., WILSON G.
	Astron. J., 131, 250-260 (2006)
	Spitzer 70 and 160 µm observations of the extragalactic First Look Survey.
o	Table 2: <FLS70 JHHMMSS.s+DDMMSS> N=845. Table 3: <FLS160 JHHMMSS.s+DDMMSS> N=227.
=E=	Catalogue in electronic form as J/AJ/131/250
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FLS70
FLS70	(First Look Survey, 70mu.m)
Write:	<<FLS70 JHHMMSS.s+DDMMSS>>
N:	845
Object:	(submm) (SIMBAD class: Infrared = Infra-Red Source)
Note:	70 mu.m observations from the Spitzer extragalactic First Look Survey.
Ref:	=2006AJ....131..250F
by	FRAYER D.T. , FADDA D., YAN L., MARLEAU F.R., CHOI P.I., HELOU G., SOIFER B.T., APPLETON P.N., ARMUS L., BECK R., DOLE H., ENGELBRACHT C.W., FANG F., GORDON K.D., HEINRICHSEN I., HENDERSON D., HESSELROTH T., IM M., KELLY D.M., LACY M., LAINE S., LATTER W.B., MAHONEY W., MAKOVOZ D., MASCI F.J., MORRISON J.E., MOSHIR M., NORIEGA-CRESPO A., PADGETT D.L., PESENSON M., SHUPE D.L., SQUIRES G.K., STORRIE-LOMBARDI L.J., SURACE J.A., TEPLITZ H.I., WILSON G.
	Astron. J., 131, 250-260 (2006)
	Spitzer 70 and 160 µm observations of the extragalactic First Look Survey.
o	Table 2: <FLS70 JHHMMSS.s+DDMMSS> N=845. Table 3: <FLS160 JHHMMSS.s+DDMMSS> N=227.
=E=	Catalogue in electronic form as J/AJ/131/250
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FLSBG
FLSBG	(Fornax Low Surface Brigtness G)
Write:	<<FLSBG NNN>>
N:	321
Object:	G in ClG (SIMBAD class: Galaxy)
in source:	NAME Fornax Cluster
Ref:	=1988MNRAS.232..239D
by	DAVIES J.I. , PHILLIPPS S., CAWSON M.G.M., DISNEY M.J., KIBBLEWHITE E.J.
	Mon. Not. R. Astron. Soc., 232, 239-258 (1988)
	Low surface brightness galaxies in the Fornax cluster: automated galaxy surface photometry. III.
o	<FLSBG NNN> (Nos 1-187)
Ref:	=1990MNRAS.245..289I
by	IRWIN M.J. , DAVIES J.I., DISNEY M.J., PHILLIPPS S.
	Mon. Not. R. Astron. Soc., 245, 289-304 (1990)
	Automated galaxy surface photometry. V. Detection of very low surface brightness galaxies.
o	Table A3: cross-id. HNN not in Simbad
o	Table A2: <FLSBG NNN> (Nos 188-321)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FLSGMRT
FLSGMRT	(First Look Survey, Giant Metrewave Radio Telescope)
Write:	<<FLSGMRT JHHMMSS.s+DDMMSS>>
N:	3944
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	GMRT 610MHz survey of the Spitzer extragalactic First Look Survey field.
Ref:	=2007MNRAS.376.1251G
by	GARN T. , GREEN D.A., HALES S.E.G., RILEY J.M., ALEXANDER P.
	Mon. Not. R. Astron. Soc., 376, 1251-1260 (2007)
	Deep 610-MHz Giant Metrewave Radio Telescope observations of the Spitzer extragalactic First Look Survey field - I. Observations, data analysis and source catalogue.
o	Catalogue: <FLSGMRT JHHMMSS.s+DDMMSS> N=3944.
=E=	Catalogue in electronic form as J/MNRAS/376/1251
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: FLSVLA
FLSVLA	(First-Look Survey, VLA)
Write:	<<FLSVLA JHHMMSS.s+DDMMSS>> <<FLSVLA GNNN>>
N:	3670
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Space Infrared Telescope Facility (SIRTF) First Look Survey (FLS): VLA catalogues. N=3565 radio components, most are distinct radio-sources. N=105 groups of two or more components, probably extended sources.
Ref:	=2003AJ....125.2411C
by	CONDON J.J. , COTTON W.D., YIN Q.F., SHUPE D.L., STORRIE-LOMBARDI L.J., HELOU G., SOIFER B.T., WERNER M.W.
	Astron. J., 125, 2411-2426 (2003)
	The SIRTF first-look survey. I. VLA image and source catalog.
o	Table 1: <FLSVLA JHHMMSS.s+DDMMSS> N=3565. Table 2: <FLSVLA GNNN> (Nos G001-G105).
=E=	Catalogue in electronic form as J/AJ/125/2411
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 1FLT
1FLT	(First Fermi/LAT Long-term gamma-ray Transient catalog)
Write:	<<1FLT JHHMM+DDMM>>
N:	142
Object:	Gamma Transient (SIMBAD class: Transient = Transient Event)
Stat:	is completely incorporated in Simbad
Note:	The ﬁrst Fermi Large Area Telescope (LAT) catalog of long-term γ-ray transient sources (1FLT) contains 142 transient γ-ray sources that are not included in the 4FGL-DR2 catalog. This comprises sources that were detected on monthly time intervals during the ﬁrst decade of Fermi-LAT operations.
Ref:	=2021ApJS..256...13B
by	BALDINI L. , BALLET J., BASTIERI D., BECERRA GONZALEZ J., BELLAZZINI R., BERRETTA A., BISSALDI E., BLANDFORD R.D., BLOOM E.D., BONINO R., BOTTACINI E., BRUEL P., BUSON S., CAMERON R.A., CARAVEO P.A., CAVAZZUTI E., CHEN S., CHIARO G., CIANGOTTINI D., CIBARIO N., CIPRINI S., CRISTARELLA ORESTANO P., CRNOGORCEVIC M., CUTINI S., D'AMMANDO F., DE LA TORRE LUQUE P., DE PALMA F., DIGEL S.W., DI LALLA N., DIRIRSA F., DI VENERE L., DOMINGUEZ A., FIORI A., FLEISCHHACK H., FRANCKOWIAK A., FUKAZAWA Y., FUNK S., FUSCO P., GARGANO F., GASPARRINI D., GERMANI S., GIGLIETTO N., GIORDANO F., GIROLETTI M., GREEN D., GRENIER I.A., GRIFFIN S., GUIRIEC S., GUSTAFSSON M., HEWITT J.W., HORAN D., IMAZAWA R., JOHANNESSON G., KERR M., KOCEVSKI D., KUSS M., LARSSON S., LATRONICO L., LI J., LIODAKIS I., LONGO F., LOPARCO F., LOVELLETTE M.N., LUBRANO P., MALDERA S., MANFREDA A., MARTI-DEVESA G., MATAKE H., MAZZIOTTA M.N., MEREU I., MEYER M., MIRABAL N., MITTHUMSIRI W., MIZUNO T., MONZANI M.E., MORSELLI A., MOSKALENKO I.V., NAGASAWA S., NEGRO M., OJHA R., ORIENTI M., ORLANDO E., PALATIELLO M., PALIYA V., PANEQUE D., PEI Z., PERSIC M., PESCE-ROLLINS M., PETROSIAN V., POON H., PORTER T.A., PRINCIPE G., RACUSIN J.L., RAINO S., RANDO R., RANI B., RAZZANO M., RAZZAQUE S., REIMER A., REIMER O., SAZ PARKINSON P.M., SCOTTON L., SERINI D., SGRO C., SISKIND E.J., SPANDRE G., SPINELLI P., SUSON D.J., TAJIMA H., TAK D., TORRES D.F., TOSTI G., TROJA E., WOOD K., YASSINE M., ZAHARIJAS G., (The Fermi-LAT Collaboration)
	Astrophys. J., Suppl. Ser., 256, 13-13 (2021)
	Catalog of long-term transient sources in the first 10 yr of Fermi-LAT data.
o	Table B1: <1FLT JHHMM+DDMM> N=142.
=E=	Catalogue in electronic form as <J/ApJS/256/13/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FLT2009]
[FLT2009]	(Fernandez+Latham+Torres+, 2009)
Write:	<<[FLT2009] T-CCCN-NNNNN>>
N:	5
Object:	EB* (SIMBAD class: EclBin = Eclipsing Binary)
Stat:	is completely incorporated in Simbad
Note:	Follow-up spectroscopy of N=5 eclipsing binary systems, discovered by the TrES survey, with the 1.5m Wyeth Reflector at the Oak Ridge Observatory (Harvard) and the 1.5m Tillinghast Reflector at the FLWO (Mount Hopkins).
Ref:	=2009ApJ...701..764F
by	FERNANDEZ J.M. , LATHAM D.W., TORRES G., EVERETT M.E., MANDUSHEV G., CHARBONNEAU D., O'DONOVAN F.T., ALONSO R., ESQUERDO G.A., HERGENROTHER C.W., STEFANIK R.P.
	Astrophys. J., 701, 764-775 (2009)
	Mass and radius determinations for five transiting M-dwarf stars.
o	Table 1: <[FLT2009] T-CCCN-NNNNN> N=5.
=E=	Catalogue in electronic form as <J/ApJ/701/764/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLV2000]
[FLV2000]	(Fiore+La Franca+Vignali+, 2000)
Write:	<<[FLV2000] PN>> <<[FLV2000] LARN>>
N:	6+7
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra hard X-ray sources, see CXOU. In PKS 0312-770 field, (Nos P1-P6). In Leonid Anti-rad field, (Nos LAR1 to LAR6).
Ref:	=2000NewA....5..143F
by	FIORE F. , LA FRANCA F., VIGNALI C., COMASTRI A., MATT G., PEROLA G.C., CAPPI M., ELVIS M., NICASTRO F.
	New Astronomy, 5, 143-153 (2000)
	Spectroscopic identification of ten faint hard X-ray sources discovered by Chandra.
o	Table 2: <[FLV2000] PN> (Nos P1-P6), <[FLV2000] LARN> (Nos LAR1-LAR6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLV2020]
[FLV2020]	(Forbrich+Lada+Viaene+, 2020) (Not yet in Simbad)
Write:	<<[FLV2020] KNNNA>>
N:	23
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	SMA observations of N=23 discrete continuum sources toward 15 [KGF2015] giant molecular clouds.
in source:	NGC 224 = M 31
Ref:	=2020ApJ...890...42F
by	FORBRICH J. , LADA C.J., VIAENE S., PETITPAS G.
	Astrophys. J., 890, 42-42 (2020)
	First resolved dust continuum measurements of individual giant molecular clouds in the Andromeda galaxy.
o	(Erratum) erratum vol. 900, art. 196 (2020)
o	Fig. 1, Table 1: <[FLV2020] KNNNA> N=23 among (Nos K026A-K026B to K291A-K291B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FLWO
FLWO	(Fred Lawrence Whipple Observatory)
*****	Avoid the usage of FLWO, prefer MLLA
Origin	of the Acronym: L (2005ApJS..160..353G)
Details on Acronym: [FLY99]
[FLY99]	(Fernandez-Soto+Lanzetta+Yahil, 1999)
Write:	<<[FLY99] Star NN>> <<[FLY99] NNNN>> <<[FLY99] A>>
N:	20+1067+6
Object:	* + G (SIMBAD class: Galaxy)
Note:	Table 2: 'Star NN', N=20 star in HDF infrared images. Table 4: N=1067 galaxies. Table 6: (Nos A-F), 6 brightest high redshift candidates in the catalogue (cross-id with format 'NNNN').
in source:	NAME HDFN
Ref:	=1999ApJ...513...34F
by	FERNANDEZ-SOTO A. , LANZETTA K.M., YAHIL A.
	Astrophys. J., 513, 34-50 (1999)
	A new catalog of photometric redshifts in the Hubble Deep Field.
o	Table 3: <[FLY99] Star NN> (Nos 1-20). Table 4: <[FLY99] NNNN> N=1067. Table 6: <[FLY99] A> (Nos A-F).
=E=	Catalogue in electronic form as J/ApJ/513/34
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FLZ2017]
[FLZ2017]	(Fritz+Linden+Zivick+, 2017)
Write:	<<[FLZ2017] NNN>>
N:	349
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Gemini-S GeMS/GSAOI spectroscopic observations of N=349 stars in the globular cluster Pyxis. Use of archival HST ACS/WFC data.
in source:	NAME Pyxis Cluster
Ref:	=2017ApJ...840...30F
by	FRITZ T.K. , LINDEN S.T., ZIVICK P., KALLIVAYALIL N., BEATON R.L., BOVY J., SALES L.V., SOHN T., ANGELL D., BOYLAN-KOLCHIN M., CARRASCO E.R., DAMKE G., DAVIES R., MAJEWSKI S., NEICHEL B., VAN DER MAREL R.
	Astrophys. J., 840, 30-30 (2017)
	The proper motion of Pyxis: the first use of Adaptive Optics in tandem with HST on a faint halo object.
o	Table 4: <[FLZ2017] NNN> N=349 among (Nos 1-421).
=E=	Catalogue in electronic form as J/ApJ/840/30
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FM
FM	(Few+Madore)
Write:	<<FM FFF-NN>>
N:	69
Object:	Ring G (SIMBAD class: Galaxy)
Note:	Catalog of Galaxies on Microfiche MN 222/1
Ref:	=1986MNRAS.222..673F
by	FEW J.M.A. , MADORE B.F.
	Mon. Not. R. Astron. Soc., 222, 673-682 (1986)
	Ring galaxies- II. Classification and statistics.
o	on microfiche MN 222/1
o	<FM FFF-NNN> N=69
Origin	of the Acronym: L = Found in the literature
Details on Acronym: FM
FM	(FitzGerald+Moffat)
*****	Avoid the usage of FM, prefer [FM74]
Origin	of the Acronym: L (1998MNRAS.297..867M)
Details on Acronym: FM
FM	(Fitzgerald+Moffat)
*****	Avoid the usage of FM, prefer [FM75]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FM2000]
[FM2000]	(Fabricius+Makarov, 2000)= ([FM2000a]) (Not yet in Simbad)
Write:	<<[FM2000] NNNNNNA>>
N:	9473+342
Object:	(SIMBAD class: = Double or Multiple Star)
Note:	Double and multiple stars in the HIPPARCOS catalogue. A letter 'A' is added at the HIP format for components identification.
Ref:	=2000A&A...356..141F
by	FABRICIUS C. , MAKAROV V.V.
	Astron. Astrophys., 356, 141-145 (2000)
	Two-colour photometry for 9473 components of close Hipparcos double and multiple stars.
o	Catalog: <[FM2000] NNNNNNA> N=9473.
Ref:	=2000A&AS..144...45F
by	FABRICIUS C. , MAKAROV V.V.
	Astron. Astrophys., Suppl. Ser., 144, 45-51 (2000)
	Hipparcos astrometry for 257 stars using Tycho-2 data.
o	Table 3: <[FM2000] NNNNNNA> N=342.
=E=	Catalogue in electronic form as J/A+A/356/141
=E=	Catalogue in electronic form as J/A+AS/144/45
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FM2000a]
[FM2000a]	(Fabricius+Makarov, 2000) (Not yet in Simbad)
*****	Avoid the usage of [FM2000a], prefer [FM2000]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FM2000b]
[FM2000b]	(Froebrich+Meusinger, 2000)
Write:	<<[FM2000b] cand N>>
N:	6
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=6 new LSB dwarf galaxies candidate in M 81 group
in source:	NAME M 81 GROUP
Ref:	=2000A&AS..145..229F
by	FROEBRICH D. , MEUSINGER H.
	Astron. Astrophys., Suppl. Ser., 145, 229-242 (2000)
	A search for LSB dwarf galaxies in the M81 group on digitally stacked Schmidt plates.
o	Table 1: <[FM2000b] cand N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FM2008]
[FM2008]	(Flaherty+Muzerolle, 2008)
Write:	<<[FM2008] NGC 2068-2071 Cluster>> <<[FM2008] NNNN>>
N:	1+67
Object:	Cluster of * + *inCl (SIMBAD class: Star)
Note:	Spitzer and MMT observations of the stellar population of a young embedded cluster associated with the NGC 2068 and 2071 reflexion nebulae.
in source:	NAME NGC 2068-2071 Cluster
Ref:	=2008AJ....135..966F
by	FLAHERTY K.M. , MUZEROLLE J.
	Astron. J., 135, 966-983 (2008)
	Evidence for early circumstellar disk evolution in NGC 2068/71.
o	Text: <[FM2008] NGC 2068-2071 Cluster> N=1. Table 2: <[FM2008] NNNN> N=69 among (Nos 17-1643).
=E=	Catalogue in electronic form as J/AJ/135/966
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FM2018]
[FM2018]	(Friedmann+Maoz, 2019)
Write:	<<[FM2018] SN FMNN>>
N:	29
Object:	Poss. SN (SIMBAD class: Supernova_Candidate = SuperNova Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=29 supernovae in eleven galaxy clusters at redshifts between 1.13 and 1.75. Use of archival data from a multi-epoch HST imaging program of a sample of twleve galaxy clusters.
Ref:	=2018MNRAS.479.3563F
by	FRIEDMANN M. , MAOZ D.
	Mon. Not. R. Astron. Soc., 479, 3563-3581 (2018)
	The rate of Type-Ia supernovae in galaxy clusters and the delay-time distribution out to redshift 1.75.
o	Fig. 2, Table 2: <[FM2018] SN FMNN> (Nos FM01-FM29).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FM74]
[FM74]	(FitzGerald+Moffat, 1974)= (FM)
Write:	<<[FM74] NNNNa>>
N:	477
Object:	* (SIMBAD class: Star)
Note:	Stars in Cl Haffner 18, Cl Haffner 19, and in the surrounding field.
in source:	Cl Haffner 18
in source:	Cl Haffner 19
Ref:	=1974AJ.....79..873F
by	FITZGERALD M.P. , MOFFAT A.F.J.
	Astron. J., 79, 873-884 (1974)
	Puppis clusters Haffner 19 and 18 ab and the 15 kiloparsec arm.
o	Table II: <[FM74] NNNN> (Nos among 1001 and 5095) = <Cl* Haffner 19 FM NNNN> (Nos 4020-4056).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FM75]
[FM75]	(Fitzgerald+Moffat, 1975)= (FM)
Write:	<<[FM75] 2483F NNN>> <<[FM75] Puppis NNN>>
N:	141+103
Object:	* (SIMBAD class: Star)
Note:	Stars in a background field '2483F' 19' south of NGC 2483, and photoelectric sequence in a 'Puppis' field at l=245deg and b=0deg. See also NGC 2483 NNN for stars in NGC 2483. See also [FWS69].
Ref:	=1975A&AS...20..289F
by	FITZGERALD M.P. , MOFFAT A.F.J.
	Astron. Astrophys., Suppl. Ser., 20, 289-304 (1975)
	On the nature of the Puppis cluster NGC 2483.
o	Table 1, Fig.1: <NGC 2483 NNN> (Nos 1-166). Table 2, Fig.2: <[FM75] 2483F NNN> (Nos 1-141). Table 3, Figs 10: <[FM75] Puppis NNN> (Nos 1-103).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMB2008]
[FMB2008]	(Fenech+Muxlow+Beswick+, 2008)
Write:	<<[FMB2008] SS.ss+SS.s>>
N:	55+4
Object:	(Radio) (SIMBAD class: Radio = Radio Source)
Note:	MERLIN 5GHz observations. Format 'SS.ss+SS.s': the complete B1950 coordinate format is 09 55 SS.s (right ascension) and +69 40 SS.s (declination). See also: [KW75], [MPW94], [MMW2002].
in source:	M82 = NGC 3034
Ref:	=2008MNRAS.391.1384F
by	FENECH D.M. , MUXLOW T.W.B., BESWICK R.J., PEDLAR A., ARGO M.K.
	Mon. Not. R. Astron. Soc., 391, 1384-1402 (2008)
	Deep MERLIN 5GHz radio imaging of supernova remnants in the M82 starburst.
o	Numbering 'NN' in Table 2, col(1) is not used in Simbad.
o	Table 2: <[FMB2008] SS.ss+SS.s> N=55.
Ref:	=2013MNRAS.431.1107G
by	GENDRE M.A. , FENECH D.M., BESWICK R.J., MUXLOW T.W.B., ARGO M.K.
	Mon. Not. R. Astron. Soc., 431, 1107-1120 (2013)
	Flux density variations of radio sources in M82 over the last three decades.
o	Table A1: <[FMB2008] SS.ss+SS.s> (Nos 42.81+59.6, 43.78+59.3, 44.28+61.1) added.
o	Calibrator 0955+697 not identified (not enough information).
=E=	Catalogue in electronic form as J/MNRAS/391/1384
=E=	Catalogue in electronic form as <J/MNRAS/431/1107/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMB91]
[FMB91]	(Fabricant+McClintock+Bautz, 1991)
Write:	<<[FMB91] NNN>>
N:	288
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Einstein Medium Sensitivity Survey. Image in Plate 1
in source:	ClG 1358+6245 = 1E 1358.4+6245
Ref:	=1991ApJ...381...33F
by	FABRICANT D.G. , McCLINTOCK J.E., BAUTZ M.
	Astrophys. J., 381, 33-54 (1991)
	Galaxy evolution in distant, X-ray selected clusters of galaxies. I. Cl 1358+6245.
o	Table 5: <[FMB91] NNN> (Nos 1-288)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FMC
FMC	(Finkezeller+Mundt, Catalogue)
Write:	<<FMC NN>>
N:	57
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Herbig Ae/Be stars.
Ref:	=1984A&AS...55..109F
by	FINKENZELLER U. , MUNDT R.
	Astron. Astrophys., Suppl. Ser., 55, 109-141 (1984)
	The Herbig Ae/Be stars associated with nebulosity.
o	BLJ 71 (FMC 56) misprint for BHJ 71 = Ass CEP OB 3-71
o	Table I: <FMC NN> (Nos 1-57).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMC2003]
[FMC2003]	(Ferrari+Maurogordato+Cappi+, 2003)
Write:	<<[FMC2003] gN>> <<[FMC2003] BCG group>> <<[FMC2003] Ridge>> <<[FMC2003] NNN>>
N:	8+191
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	ESO 3.6m telescope and CFHT observations. N=8 sub-groups in ACO 521, (Nos g1-g6), BCG group (Bright Cluster Galaxy = [MPB2000] 49), and Ridge. N=191 galaxies in ACO 521. See also [MPB2000].
in source:	ACO 521
Ref:	=2003A&A...399..813F
by	FERRARI C. , MAUROGORDATO S., CAPPI A., BENOIST C.
	Astron. Astrophys., 399, 813-828 (2003)
	Multiple merging events in Abell 521.
o	Fig.1: <[FMC2003] gN> (Nos g1-g6), <[FMC2003] BCG group> N=1, <[FMC2003] Ridge> N=1. Table 10: <[FMC2003] NNN> (Nos 1-191).
=E=	Catalogue in electronic form as J/A+A/399/813
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMC2004]
[FMC2004]	(Fassnacht+Moustakas+Casertano+, 2004)
Write:	<<[FMC2004] GDS JHHMMSS+DDMMSS>>
N:	48
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	GOODS (Great Observatories Origins Deep Survey) HST ACS observations. Search for lens candidate galaxies. N=25 candidates are found in the GOODS South Field, and N=23 in the GOODS North Field.
in source:	NAME GOODS North Field
in source:	NAME GOODS South Field
Ref:	=2004ApJ...600L.155F
by	FASSNACHT C.D. , MOUSTAKAS L.A., CASERTANO S., FERGUSON H.C., LUCAS R.A., PARK Y.
	Astrophys. J., 600, 155-158 (2004)
	Strong gravitational lens candidates in the GOODS ACS fields.
o	Table 1: <[FMC2004] GDS JHHMMSS+DDMMSS> N=48.
=E=	Catalogue in electronic form as J/ApJ/600/L155
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMC99]
[FMC99]	(Fuchs+Mirabel+Chaty+, 1999)
Write:	<<[FMC99] A>>
N:	6+1
Object:	(IR) + * (SIMBAD class: Infrared = Infra-Red Source)
Note:	ISO observations of the cloud SGR 1806-20. (Nos A, C-F) are stars in or behind the cloud. (No. B) is a Cl*. (No. O) is the LBV star supposed to be the IR counterpart of NAME SGR 1806-20. See also [EGH2001], [EGH2001b].
in source:	NAME Sgr 1806-20
Ref:	=1999A&A...350..891F
by	FUCHS Y. , MIRABEL F., CHATY S., CLARET A., CESARSKY C.J., CESARSKY D.A.
	Astron. Astrophys., 350, 891-899 (1999)
	ISO observations of the environment of the soft γ-ray repeater SGR 1806-20.
o	Figs 2, 4: <[FMC99] A> (Nos A-F, O).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMD2013]
[FMD2013]	(Farina+Montuori+Decarli+, 2013)
Write:	<<[FMD2013] QQQ J1519+0627>>
N:	1
Object:	Triple quasar (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	ESO NTT EFOSC2 spectroscopy and Calar Alto 3.5m telescope NIR photometry of a triple quasar.
Ref:	=2013MNRAS.431.1019F
by	FARINA E.P. , MONTUORI C., DECARLI R., FUMAGALLI M.
	Mon. Not. R. Astron. Soc., 431, 1019-1025 (2013)
	Caught in the act: discovery of a physical quasar triplet.
o	<[FMD2013] QQQ J1519+0627> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMD2015]
[FMD2015]	(Fu+Myers+Djorgovski+, 2015)
Write:	<<[FMD2015] JHHMMSS.ss+DDMMSS.s>> <<[FMD2015] JHHMM+DDMM>> <<[FMD2015] HHMMSS.ss+DDMMSS.s>> (not recognised by Simbad, but found in literature) <<[FMD2015] HHMM+DDMM>>
N:	104+6
Object:	AGN + Pair of AGNs (SIMBAD class: Radio = Radio Source)
Note:	Keck I LRIS spectroscopy of N=104 radio-selected AGNs and N=6 confirmed pairs of AGNs. Use of VLA and SDSS Stripe 82 data.
Ref:	=2015ApJ...799...72F
by	FU H. , MYERS A.D., DJORGOVSKI S.G., YAN L., WROBEL J.M., STOCKTON A.
	Astrophys. J., 799, 72 (2015)
	Radio-selected binary active galactic nuclei from the Very Large Array Stripe 82 survey.
o	Tables 1-3: <[FMD2015] JHHMMSS.ss+DDMMSS.s> N=104. Table 3: <[FMD2015] JHHMM+DDMM> N=6.
=E=	Catalogue in electronic form as J/ApJ/799/72
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FMF
FMF	(Fast-Moving Flocculi)
Write:	<<FMF NN>> <<FMF SE>>
N:	15+1
Object:	Flocculi (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-15): Fast-Moving Flocculi in Cas A. p.L91 and Plate L9: FMF 118-121 are an extension of jet emission knots from Kamper and Van Den Bergh (1976), so they are named 'KB MK NNN' in SIMBAD. FMF SE = one suspected Fast-Moving Flocculi in the South East. See also [FG96] and [FHM2006].
in source:	NAME Cas A
Ref:	=1987ApJ...313..378F
by	FESEN R.A. , BECKER R.H., BLAIR W.P.
	Astrophys. J., 313, 378-388 (1987)
	Discovery of fast-moving nitrogen-rich ejecta in the supernova remnant Cassiopeia A.
o	Table 1: <FMF N> (Nos 1-9), <FMF SE>
Ref:	=1988ApJ...329L..89F
by	FESEN R.A. , BECKER R.H., GOODRICH R.W.
	Astrophys. J., 329, 89-92 (1988)
	Highest velocity ejecta of Cassiopeia A.
o	Table 1: <FMF NN> (Nos 10-15) added. p.L91: <KB MK NNN> (Nos 118-121) added.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FMF
FMF	(Fast-Moving Flocculi)
*****	Avoid the usage of FMF, prefer KB
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FMG99]
[FMG99]	(Figer+Morris+Geballe+, 1999)
Write:	<<[FMG99] N>>
N:	8
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Note:	HST NICMOS observations.
in source:	NAME Pistol Nebula
Ref:	=1999ApJ...525..759F
by	FIGER D.F. , MORRIS M., GEBALLE T.R., RICH R.M., SERABYN E., McLEAN I.S., PUETTER R.C., YAHIL A.
	Astrophys. J., 525, 759-771 (1999)
	High-resolution infrared imaging and spectroscopy of the Pistol nebula: evidence for ejection.
o	Table 5: <[FMG99] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMI2018]
[FMI2018]	(Frayer+Maddalena+Ivison+, 2018) (Not yet in Simbad)
Write:	<<[FMI2018] SMM J02399-0136 W1>>
N:	1
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	GBT (CO(1-0), CO(3-2), and CO(7-6)) and ALMA (CO(3-2) and CO(7-6)) observations of N=1 extended component of molecular gas in [BCS98] SMM J02399-0136. See also [ISL98].
in source:	[BCS98] SMM J02399-0136
Ref:	=2018ApJ...860...87F
by	FRAYER D.T. , MADDALENA R.J., IVISON R.J., SMAIL I., BLAIN A.W., VANDEN BOUT P.
	Astrophys. J., 860, 87-87 (2018)
	The discovery of a new massive molecular gas component associated with the submillimeter galaxy SMM J02399-0136.
o	<[FMI2018] SMM J02399-0136 W1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMJ2014]
[FMJ2014]	(Foley+McCully+Jha+, 2014)
Write:	<<[FMJ2014] S1>>
N:	1
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations of N=1 point source near the position of SN 2008ha.
in source:	SN 2008ha
Ref:	=2014ApJ...792...29F
by	FOLEY R.J. , McCULLY C., JHA S.W., BILDSTEN L., FONG W.-F., NARAYAN G., REST A., STRITZINGER M.D.
	Astrophys. J., 792, 29 (2014)
	Possible detection of the stellar donor or remnant for the type Iax supernova 2008ha.
o	Fig. 1: <[FMJ2014] S1> (No S1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FMK
FMK	(Fast-Moving Knot) (Not yet in Simbad)
*****	Avoid the usage of FMK, prefer [GF2001]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FMK
FMK	(Fast-Moving Knot)
*****	Avoid the usage of FMK, prefer [HF96]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FMK2006]
[FMK2006]	(Fassnacht+McKean+Koopmans+, 2006)= (ACS)
Write:	<<[FMK2006] ACS JHHMMSS+DDMM>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Discovery of 2 strong lens candidates in deep images obtained with the Advanced Camera for Surveys (ACS) on the HST. Additional Keck LRIS and Gemini GMOS spectroscopy. See also [KF99] and [MFD95].
Ref:	=2006ApJ...651..667F
by	FASSNACHT C.D. , McKEAN J.P., KOOPMANS L.V.E., TREU T., BLANDFORD R.D., AUGER M.W., JELTEMA T.E., LUBIN L.M., MARGONINER V.E., WITTMAN D.
	Astrophys. J., 651, 667-675 (2006)
	Three gravitational lenses for the price of one: enhanced strong lensing through galaxy clustering.
o	Table 2, Fig.2: <[FMK2006] ACS JHHMMSS+DDMM> N=2, respectively = <NAME FRED>, <NAME GINGER>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FML2001]
[FML2001]	(Finger+Macomb+Lamb+, 2001)
Write:	<<[FML2001] A>>
N:	4
Object:	* (SIMBAD class: Star)
Note:	SAAO observations of the field around RX J0052.1-7319. (Nos A-D), N=4 stars.
Ref:	=2001ApJ...560..378F
by	FINGER M.H. , MACOMB D.J., LAMB R.C., PRINCE T.A., COE M.J., HAIGH N.J.
	Astrophys. J., 560, 378-383 (2001)
	Discovery of pulsed x-rays from the SMC transient RX J0052.1-7319.
o	Fig.6: <[FML2001] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FML2002]
[FML2002]	(Fang+Marshall+Lee+, 2002)
Write:	<<[FML2002] QSO J2158-3013 abs N.NNNN>>
N:	1
Object:	Absorber
Note:	Chandra observations of a O VIII Ly-alpha absorber in the line of sight of PKS 2155-304 = QSO J2158-3013.
Ref:	=2002ApJ...572L.127F
by	FANG T. , MARSHALL H.L., LEE J.C., DAVIS D.S., CANIZARES C.R.
	Astrophys. J., 572, 127-130 (2002)
	Chandra detection of O VIII Lyα absorption from an overdense region in the intergalactic medium.
o	<[FML2002] QSO J2158-3013 abs N.NNNN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FML2007]
[FML2007]	(France+McCandliss+Lupu, 2007) (Not yet in Simbad)
Write:	<<[FML2007] SW>> <<[FML2007] A>> <<[FML2007] A>> <<[FML2007]* A**>>
N:	3+2+2
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Spitzer observations of IC 405: Bow shock structure (Nos SE, SC, SW), and Nebular filaments (Nos A-B), filament A broken in 3 sub-regions A, A, A*.
in source:	IC 405
Ref:	=2007ApJ...655..920F
by	FRANCE K. , McCANDLISS S.R., LUPU R.E.
	Astrophys. J., 655, 920-939 (2007)
	A cometary bow shock and mid-infrared emission variations revealed in Spitzer observations of HD 34078 and IC 405.
o	Figs 4, 5, Table 1: <[FML2007] SW> (Nos SE, SC, SW). Figs 2, 3, Table 2: <[FML2007] A> (Nos A-B), <[FML2007] A> N=1, <[FML2007] A*> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FML2008]
[FML2008]	(Ford+McClure-Griffiths+Lockman+, 2008)
Write:	<<[FML2008] LLL.ll+BB.bb>>
N:	403
Object:	HI Cloud (SIMBAD class: HI = HI (21cm) Source)
Note:	Parkes Radio Telescope multi-beam receiver HI observations. Galactic All-Sky Survey pilot project.
Ref:	=2008ApJ...688..290F
by	FORD H.A. , McCLURE-GRIFFITHS N.M., LOCKMAN F.J., BAILIN J., CALABRETTA M.R., KALBERLA P.M.W., MURPHY T., PISANO D.J.
	Astrophys. J., 688, 290-305 (2008)
	H I clouds in the lower halo. I. The Galactic All-Sky Survey pilot region.
o	(Erratum) erratum vol. 710, p. 1868 (2010)
o	Table 1: <[FML2008] LLL.ll+BB.bb> N=403.
=E=	Catalogue in electronic form as <J/ApJ/688/290/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FMM
FMM	(Figer+McLean+Morris)
*****	Avoid the usage of FMM, prefer qF
Origin	of the Acronym: L (1999MNRAS.304L..10G)
Details on Acronym: [FMM2002]
[FMM2002]	(Feldmeier+Mihos+Morrison+, 2002)
Write:	<<[FMM2002] A1413 arc N>> <<[FMM2002] MKW7 arc N>>
N:	5+1
Object:	Arc (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Kitt Peak observations. Tidal debris arcs in ACO 1413 and MKW 7.
in source:	ACO 1413
in source:	MKW 7
Ref:	=2002ApJ...575..779F
by	FELDMEIER J.J. , MIHOS J.C., MORRISON H.L., RODNEY S.A., HARDING P.
	Astrophys. J., 575, 779-800 (2002)
	Deep CCD surface photometry of galaxy clusters. I. Methods and initial studies of intracluster starlight.
o	Table 4, Figs 23, 24: <[FMM2002] A1413 arc N> (Nos 1-5), <[FMM2002] MKW7 arc N> (No. 1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMM2009]
[FMM2009]	(Feigeslon+Martin+McNeill+, 2009)
Write:	<<[FMM2009] XA>>
N:	10
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Chandra observations of NGC 6334.
in source:	NGC 6334
Ref:	=2009AJ....138..227F
by	FEIGELSON E.D. , MARTIN A.L., McNEILL C.J., BROOS P.S., GARMIRE G.P.
	Astron. J., 138, 227-239 (2009)
	Stellar clusters in the NGC 6334 star-forming complex.
o	NGC 6634 in Introduction, and in paragraphs 2.2 and 3.5 is a misprint for NGC 6334.
o	Table 2, Fig. 5: <[FMM2009] XA> (Nos XA-XJ).
=E=	Catalogue in electronic form as <J/AJ/138/227/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMM2014]
[FMM2014]	(Fujii+Minamidani+Mizuno+, 2014) (Not yet in Simbad)
Write:	<<[FMM2014] NNN NN>>
N:	18+3
Object:	Clump (SIMBAD class: denseCore = Dense Core)
Note:	12CO(J=3-2, 1-0) and 13CO(J=1-0) observations of N=18+3 clumps in LHA 120-N 48 and N 49 with the ASTE and Mopra telescopes.
in source:	Magellanic Clouds:LMC:LHA 120-N 48 = LHA 120-N 48
in source:	Magellanic Clouds:LMC:LHA 120-N 49 = LHA 120-N 49
Ref:	=2014ApJ...796..123F
by	FUJII K. , MINAMIDANI T., MIZUNO N., ONISHI T., KAWAMURA A., MULLER E., DAWSON J., TATEMATSU K., HASEGAWA T., TOSAKI T., MIURA R.E., MURAOKA K., SAKAI T., TSUKAGOSHI T., TANAKA K., EZAWA H., FUKUI Y.
	Astrophys. J., 796, 123 (2014)
	Dense molecular clumps associated with the Large Magellanic Cloud supergiant shells LMC 4 and LMC 5.
o	Table 3, col(1): <[FMM2014] NNN NN> (Nos N48-1 to N48-18, N49-1 to N49-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMM95]
[FMM95]	(Figer+McLean+Morris, 1995)
Write:	<<[FMM95] N>>
N:	3
Object:	* (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Note:	Table 1: [FMM95] N are respectively star 1, 2, and 3 for the authors.
Ref:	=1995ApJ...447L..29F
by	FIGER D.F. , McLEAN I.S., MORRIS M.
	Astrophys. J., 447, 29-32 (1995)
	Two new Wolf-Rayet stars and a luminous blue variable star in the Quintuplet (AFGL 2004) near the Galactic Center.
o	q1 = MGM 5-1, q8 = MGM 5-8, q10 = MGM 5-10
o	Table 1: <[FMM95] N> (Nos 1-3)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMN2004]
[FMN2004]	(Felli+Massi+Navarrini+, 2006)
Write:	<<[FMN2004] CVV>>
N:	2
Object:	Core (SIMBAD class: PartofCloud = Part of Cloud)
Note:	HCO+ cores in 2 maps at velocities -17km.s(-1) (Core C17) and -19km.s(-1) (Core C19) in the SH 2-235 A-B star forming region. See also [FMR2006b].
in source:	NAME SH 2-235 A-B
Ref:	=2004A&A...420..553F
by	FELLI M. , MASSI F., NAVARRINI A., NERI R., CESARONI R., JENNESS T.
	Astron. Astrophys., 420, 553-569 (2004)
	New light on the S235A-B star forming region.
o	Fig.1: Maser = [BE83] Maser 173.72+02.70, source M 1 = [FTV97] M1. IRAS 20126+4140 is a misprint for IRAS 20126+4104.
o	Fig.6: <[FMN2004] CVV> (Nos C17, C19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMP2006]
[FMP2006]	(Frinchaboy+Munoz+Phelps+, 2006)= ([FMP2006a])
Write:	<<[FMP2006] NNN>>
N:	11
Object:	* (SIMBAD class: Star)
Note:	Photometry at the University of Virginia's 40 inch telescope. Spectroscopy at the 4m Blanco telescope at CTIO. Stellar velocities of stars in the fields of vdB-Hagen 176, Berkeley 29, and Saurer 1.
in source:	[SSW94] a
Ref:	=2006AJ....131..922F
by	FRINCHABOY P.M. , MUNOZ R.R., PHELPS R.L., MAJEWSKI S.R., KUNKEL W.E.
	Astron. J., 131, 922-938 (2006)
	Photometry and spectroscopy of old, outer disk star clusters: vdB-Hagen 176, Berkeley 29, and Saurer 1.
o	Saurer 1 = [SSW94] a.
o	Table 6: <Cl* VDBH 176 FMP NNNNN> N=19 among (Nos 140-15302). Table 7: <Cl* Berkeley 20 FMP NNNNN> N=20 among (Nos 10308-11285). Table 8: <Cl* Berkeley 29 FMP NNNN> N=25 among (Nos 201-1461). Table 9: <Cl* Berkeley 39 FMP NNNNN> N=54 among (Nos 20289-23082). Table 10: <[FMP2006] NNN> N=11 among (Nos 122-706).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMP2006a]
[FMP2006a]	(Frinchaboy+Munoz+Phelps+, 2006)
*****	Avoid the usage of [FMP2006a], prefer [FMP2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMP2006b]
[FMP2006b]	(Frew+Madsen+Parker, 2006)= (Fr)
Write:	<<[FMP2006b] Fr 2-NN>>
N:	25
Object:	Gal. Nebula (SIMBAD class: GalNeb = Nebula)
Note:	N=25 Hα nebulae discovered from the Southern Hα Sky Survey (SHASSA) and the Virginia Tech Spectral line Survey (VTSS).
Ref:	=2006IAUS..234..395F
by	FREW D.J. , MADSEN G.J., PARKER Q.A.
	IAUS, 234, 395 (2006)
	Search for new emission nebulae from the SHASSA and VTSS surveys.
o	Table 1: <[FMP2006b] Fr 2-NN> (Nos 2-1 to 2-18).
Ref:	=2013MNRAS.431....2F
by	FREW D.J. , BOJICIC I.S., PARKER Q.A.
	Mon. Not. R. Astron. Soc., 431, 2-26 (2013)
	A catalogue of integrated Hα fluxes for 1258 Galactic planetary nebulae.
o	Tables 1+4: <[FMP2006b] Fr 2-NN> (Nos 2-23 to 2-27) added.
=E=	Catalogue in electronic form as <J/MNRAS/431/2/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMR2006]
[FMR2006]	(Figer+MacKenty+Robberto+, 2006)= ([FMR2006a])
Write:	<<[FMR2006] NN>>
N:	16
Object:	*inCl (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	KPNO-IRMOS, 2MASS and Spitzer observations: N=16 supergiant stars in the massive stellar cluster [BDS2003] 122.
in source:	[BDS2003] 122
Ref:	=2006ApJ...643.1166F
by	FIGER D.F. , MacKENTY J.W., ROBBERTO M., SMITH K., NAJARRO F., KUDRITZKI R.P., HERRERO A.
	Astrophys. J., 643, 1166-1179 (2006)
	Discovery of an extraordinarily massive cluster of red supergiants.
o	(Erratum) Erratum vol. 646, p.1452 (2006)
o	Massive star cluster in the title is [BDS2003] 122
o	Table 1: <[FMR2006] NN> (Nos 1-15).
Ref:	=2006ApJ...647L.139N
by	NAKASHIMA J.-I. , DEGUCHI S.
	Astrophys. J., 647, 139-142 (2006)
	SiO masers in a Scutum massive star cluster of red supergiants.
o	Table 1, text: <[FMR2006] NN> (Nos 16-17) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMR2006a]
[FMR2006a]	(Figer+MacKenty+Robberto+, 2006)
*****	Avoid the usage of [FMR2006a], prefer [FMR2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMR2006b]
[FMR2006b]	(Felli+Massi+Robberto, 2006)
Write:	<<[FMR2006b] IR NN>> <<[FMR2006b] VLA N>> <<[FMR2006b] H2O-N>>
N:	15+2+3
Object:	(IR) + (Rad) + H2O Maser (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC archive data of the star forming region SH 2-235 A-B. See also [FMN2004].
in source:	NAME SH 2-235 A-B
Ref:	=2006A&A...453..911F
by	FELLI M. , MASSI F., ROBBERTO M., CESARONI R.
	Astron. Astrophys., 453, 911-922 (2006)
	New signposts of massive star formation in the S235A-B region.
o	Fig.2, Table 2: <[FMR2006b] IR NN> (Nos 1-15). Fig.5, Table 3: <[FMR2006b] VLA N> (Nos 1-2). Fig.6, Table 4: <[FMR2006b] H2O-N> (Nos 1-3).
=E=	Catalogue in electronic form as J/A+A/453/911
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMR2009]
[FMR2009]	(Franco-Hernandez+Moran+Rodriguez+, 2009)
Write:	<<[FMR2009] East>> <<[FMR2009] West>>
N:	2
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	SMA 1.3mm dust continuum observations toward the massive star formation region IRAS 16547-4247.
Ref:	=2009ApJ...701..974F
by	FRANCO-HERNANDEZ R. , MORAN J.M., RODRIGUEZ L.F., GARAY G.
	Astrophys. J., 701, 974-983 (2009)
	The rotating molecular structures and the ionized outflow associated with IRAS 16547-4247.
o	Table 2: <[FMR2009] East>, <[FMR2009] West>, N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMS2000]
[FMS2000]	(Flaccomio+Micela+Sciortino+, 2000)= (FX)
Write:	<<[FMS2000] XNNN>>
N:	169
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations towards the star forming region NGC 2264. Finding chart in Figs A1.
in source:	NGC 2264
Ref:	=2000A&A...355..651F
by	FLACCOMIO E. , MICELA G., SCIORTINO S., DAMIANI F., FAVATA F., HARNDEN F.R.Jr, SCHACHTER J.
	Astron. Astrophys., 355, 651-667 (2000)
	HRI observations of PMS stars in NGC 2264.
o	Table 3: cross-id MX, from Young private, not in SIMBAD.
o	Table 3: <[FMS2000] XNNN> (Nos X1-X169).
=E=	Catalogue in electronic form as J/A+A/355/651
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMS2001]
[FMS2001]	(Font+Mitchell+Sandell, 2001)
Write:	<<[FMS2001] NGC 7129 CON>> <<[FMS2001] LkHa 234 SMM N>>
N:	4+2
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=4 13CO peaks assumed to be physical clumps in NGC 7129. Table 4: N=2 smm sources in EM* LkHa 234, embedded in NGC 7129.
in source:	NGC 7129
Ref:	=2001ApJ...555..950F
by	FONT A.S. , MITCHELL G.F., SANDELL G.
	Astrophys. J., 555, 950-960 (2001)
	A submillimeter study of the star-forming region NGC 7129.
o	Table 1: <[FMS2001] NGC 7129 CON> (Nos CO1 to CO4). Table 4: <[FMS2001] LkHa 234 SMM N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMS2006]
[FMS2006]	(Flaccomio+Micela+Sciortino, 2006)= (ACIS)
Write:	<<[FMS2006] NNN>>
N:	420
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS observations of the field of NGC 2264. See also Cl* NGC 2264 FMS 2-NNNN for the objects in Table 3.
in source:	NGC 2264
Ref:	=2006A&A...455..903F
by	FLACCOMIO E. , MICELA G., SCIORTINO S.
	Astron. Astrophys., 455, 903-921 (2006)
	ACIS-I observations of NGC 2264. Membership and X-ray properties of PMS stars.
o	Table 1: <[FMS2006] NNN> (Nos 1-420). Table 3: <Cl* NGC 2264 FMS 2-NNNN> (Nos 2-1 to 2-1598).
=E=	Catalogue in electronic form as J/A+A/455/903
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMS2007]
[FMS2007]	(Ferrarese +Mould+Stetson+, 2007)
Write:	<<[FMS2007] CNN>> <<[FMS2007] PC xxx.x-yyy.y>> <<[FMS2007] WFN xxx.x-yyy.y>> <<[FMS2007] VNN>>
N:	56+176+70
Object:	Cepheid + * + V* (SIMBAD class: Star)
Stat.	in SIMBAD: Tables 5 and 11 are completely incorporated.
Note:	HST WFPC2 observations of NGC 5128.
in source:	NGC 5128
Ref:	=2007ApJ...654..186F
by	FERRARESE L. , MOULD J.R., STETSON P.B., TONRY J.L., BLAKESLEE J.P., AJHAR E.A.
	Astrophys. J., 654, 186-218 (2007)
	The discovery of Cepheids and a distance to NGC 5128.
o	Table 5: <[FMS2007] CNN> (Nos C1-C56). Table 8: <[FMS2007] PC xxx.x-yyy.y> N=36, <[FMS2007] WFN xxx.x-yyy.y> N=140. Table 11: <[FMS2007] VNN> (Nos V1-V70).
=E=	Catalogue in electronic form as J/ApJ/654/186
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMS2013]
[FMS2013]	(Friesen+Medeiros+Schnee+, 2013)
Write:	<<[FMS2013] Na>>
N:	11
Object:	Clump (SIMBAD class: denseCore = Dense Core)
Note:	GBT KFPA observations of N=11 HC7N clumps towards the Serpens South cluster.
in source:	NAME Serpens South Cluster
Ref:	=2013MNRAS.436.1513F
by	FRIESEN R.K. , MEDEIROS L., SCHNEE S., BOURKE T.L., DI FRANCESCO J., GUTERMUTH R., MYERS P.C.
	Mon. Not. R. Astron. Soc., 436, 1513-1529 (2013)
	Abundant cyanopolyynes as a probe of infall in the Serpens south cluster-forming region.
o	Fig. 1, Table 2: <[FMS2013] Na> N=11 among (Nos 1a-1b to 7a-7b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMS2015]
[FMS2015]	(Franck+McGaugh+Schombert, 2015)
Write:	<<[FMS2015] CL J0442 NN>> <<[FMS2015] 3C 068.2 NN>> <<[FMS2015] MS 1426 NN>>
N:	48+31+33
Object:	G (SIMBAD class: Galaxy)
Note:	KPNO Mayall 4-m SQIID and NEWFIRM observations of N=48+31+33 galaxies in the field of the three radio-loud sources MITG J044226+0202, 3C 68.2, and 1E 1426.9+1052.
Ref:	=2015AJ....150...46F
by	FRANCK J.R. , McGAUGH S.S., SCHOMBERT J.M.
	Astron. J., 150, 46 (2015)
	Three candidate clusters around high redshift radio-loud sources: MG1 J04426+0202, 3C 068.2, and MS 1426.9+1052.
o	Table 3: <[FMS2015] CL J0442 NN> (Nos 1-48). Table 4: <[FMS2015] 3C 068.2 NN> (Nos 1-31). Table 5: <[FMS2015] MS 1426 NN> (Nos 1-33).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMT2002]
[FMT2002]	(Fynbo+Moller+Thomsen+, 2002) (Not yet in Simbad)
Write:	<<[FMT2002] MDD-NN>>
N:	11+8
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=11 and 8 respectively candidate LEGOs (Ly-alpha Emitting Galaxy-building Object) in the fields of GRB 000301C (301 in the format) and GRB 000926 (926 in the format. See also [FJM2003], [JBF2005], LEGO.
Ref:	=2002A&A...388..425F
by	FYNBO J.P.U. , MOLLER P., THOMSEN B., HJORTH J., GOROSABEL J., ANDERSEN M.I., EGHOLM M.P., HOLLAND S., JENSEN B.L., PEDERSEN H., WEIDINGER M.
	Astron. Astrophys., 388, 425-438 (2002)
	Deep Lyα imaging of two z = 2.04 GRB host galaxy fields.
o	Tables 2, 3, Fig.5: <[FMT2002] 301-NN> N=11, <[FMT2002] 926-N> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMT2003]
[FMT2003]	(Fukui+Moriguchi+Tamura+, 2003)
Write:	<<[FMT2003] Peak A>>
N:	4
Object:	CO peak (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Nanten telescope CO(1-0) observations of CO peaks in SNR 347.3-0.5. See also [MTT2005b].
in source:	SNR G347.3-00.5
Ref:	=2003PASJ...55L..61F
by	FUKUI Y. , MORIGUCHI Y., TAMURA K., YAMAMOTO H., TAWARA Y., MIZUNO N., ONISHI T., MIZUNO A., UCHIYAMA Y., HIRAGA J., TAKAHASHI T., YAMASHITA K., IKEUCHI S.
	Publ. Astron. Soc. Jap., 55, 61-64 (2003)
	Discovery of interacting molecular gas toward the TeV γ-ray peak of the SNR G 347.3-0.5.
o	Fig.2: <[FMT2003] Peak A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMT2009]
[FMT2009]	(Faustini+Molinari+Testi+, 2009)
Write:	<<[FMT2009] NNNA>>
N:	23
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Palomar 60-in telescope and NTT SOFI NIR observations of N=23 young stellar clusters associated with 22 high-mass protostellar candidates (see also Mol).
Ref:	=2009A&A...503..801F
by	FAUSTINI F. , MOLINARI S., TESTI L., BRAND J.
	Astron. Astrophys., 503, 801-816 (2009)
	Properties of stellar clusters around high-mass young stars.
o	Table 2: <[FMT2009] NNNA> N=23 among (Nos 3-160).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMT2010]
[FMT2010]	(Fiorentino+Monachesi+Trager+, 2010)
Write:	<<[FMT2010] FF NN>>
N:	17+14
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Stat:	is completely incorporated in Simbad
Note:	HST ACS/HRC observations of two fields near M32.
in source:	M 31 = NGC 224
in source:	M 32
Ref:	=2010ApJ...708..817F
by	FIORENTINO G. , MONACHESI A., TRAGER S.C., LAUER T.R., SAHA A., MIGHELL K.J., FREEDMAN W., DRESSLER A., GRILLMAIR C., TOLSTOY E.
	Astrophys. J., 708, 817-833 (2010)
	RR Lyrae variables in M32 and the disk of M31.
o	Fig. 2, Table 2: <[FMT2010] F1 NN> (Nos F1 1 to F1 17). Fig. 3, Table 3: <[FMT2010] F2 NN> (Nos F2 1 to F2 14).
=E=	Catalogue in electronic form as <J/ApJ/708/817/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMT2012]
[FMT2012]	(Fabrizio+Merle+Thevenin+, 2012)
Write:	<<[FMT2012] Car-NN>>
N:	48
Object:	RGB* (SIMBAD class: RGB* = Red Giant Branch star)
Note:	N=46 red giant and N=2 candidate carbon stars in the Carina dwarf galaxy. Use of VLT UVES and FLAMES/GIRAFFE-UVES archival data.
in source:	NAME Carina Dwarf Galaxy
Ref:	=2012PASP..124..519F
by	FABRIZIO M. , MERLE T., THEVENIN F., NONINO M., BONO G., STETSON P.B., FERRARO I., IANNICOLA G., MONELLI M., WALKER A.R., BUONANNO R., CAPUTO F., CORSI E., DALL'ORA M., DEGL'INNOCENTI S., FRANCOIS P., GILMOZZI R., MARCONI M., PITRINFERNI A., PRADA MORONI P.G., PRIMAS F., PULONE L., RIPEPI V., ROMANIELLO M.
	PASP, 124, 519-534 (2012)
	The Carina Project. V. The impact of NLTE effects on the iron content.
o	Table 1: <[FMT2012] Car-NN> N=48 among (Nos 2-55).
=E=	Catalogue in electronic form as <J/PASP/124/519/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMT92]
[FMT92]	(Falomo+Melnick+Tanzi, 1992)
Write:	<<[FMT92] AN>> <<[FMT92] BN>>
N:	5
Object:	Poss. G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ESO NTT and HST observations. Faint resolved structures, probably faint galaxies in the field of PKS 0537-441. See also [SFK88b].
Ref:	=1992A&A...255L..17F
by	FALOMO R. , MELNICK J., TANZI E.G.
	Astron. Astrophys., 255, 17-19 (1992)
	PKS 0537-441: an elusive case of a gravitationally lensed blazar.
o	G1 = [SFK88b] G1.
o	Fig.1: <[FMT92] AN> (Nos A1-A3).
Ref:	=2000ApJ...528..650L
by	LEWIS G.F. , IBATA R.A.
	Astrophys. J., 528, 650-654 (2000)
	An investigation of gravitational lensing in the southern BL Lac PKS 0537-441.
o	G1 = [SFK88b] G1.
o	Fig.3: <[FMT92] AN> (No.B1) added.
Ref:	=2003A&A...406..565H
by	HEIDT J. , JAEGER K., NILSSON K., HOPP U., FRIED J.W., SUTORIUS E.
	Astron. Astrophys., 406, 565-577 (2003)
	PKS 0537-441: Extended [OII] emission and a binary QSO?
o	Fig.1: <[FMT92] AN> (No. B2) added. Table 1: <[HJN2003] aNNa> N=18+18.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMV2006]
[FMV2006]	(Fasano+Marmo+Varela+, 2006)= (ACO)
Write:	<<[FMV2006] ANNNNa>>
N:	5+1
Object:	Cl of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Subclusters in the WINGS galaxy cluster sample.
Ref:	=2006A&A...445..805F
by	FASANO G. , MARMO C., VARELA J., D'ONOFRIO M., POGGIANTI B.M., MOLES M., PIGNATELLI E., BETTONI D., KJAERGAARD P., RIZZI L., COUCH W.J., DRESSLER A.
	Astron. Astrophys., 445, 805-817 (2006)
	WINGS: a WIde-field Nearby Galaxy-cluster Survey. I. Optical imaging.
o	Table 5: <[FMV2006] ANNNNa> N=5.
Ref:	=2009A&A...501..851V
by	VALENTINUZZI T. , WOODS D., FASANO G., RIELLO M., D'ONOFRIO M., VARELA J., BETTONI D., CAVA A., COUCH W.J., DRESSLER A., FRITZ J., MOLES M., OMIZZOLO A., POGGIANTI B.M., KJAERGAARD P.
	Astron. Astrophys., 501, 851-864 (2009)
	WINGS: a WIde-field nearby galaxy-cluster survey. III. Deep near-infrared photometry of 28 nearby clusters.
o	Table 3: <[FMV2006] ANNNNa> (No. A957x) added.
=E=	Catalogue in electronic form as J/A+A/501/851
Details on Acronym: [FMW99]
[FMW99]	(Fynbo+Moller+Warren, 1999)
Write:	<<[FMW99] psf A>> <<[FMW99] SN>> <<[FMW99] gA>> <<[FMW99] HGa>> <<[FMW99] s>>
N:	2+2+2+2+2+1
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Study of the field of QSO 0151+048. 1999MNRAS.305..849F, Table 3, text: QSO 0151+048A and B is a QSO pair, (here qA and qB, not used). N=3 stars, 'psf A' and 'psf B' (point source function), and another one 's'. N=2 sources, 'S4' and 'S5' (S5 is a galaxy), and N=1 source 's'. N=2 faint galaxies 'gA' and 'gB'. 2000A&A...358...88F, Table 3: Host galaxies (Nos HGa, HGb) respectively of QSO 0151+048A and B. The authors used the same numbering (Nos S1-S12) in 3 papers: (Nos S1-S3) are '[MW93] SN', in the field of QSO 0528-250. (Nos S4-S5) are '[FMW99] SN', in the field of QSO 0151+048. (Nos S6-S13) are '[FTM2000] SNN', in the field of QSO 1205-30. See also [MW93], [FTM2000].
Ref:	=1999MNRAS.305..849F
by	FYNBO J.U. , MOLLER P., WARREN S.J.
	Mon. Not. R. Astron. Soc., 305, 849-858 (1999)
	Extended Ly-α emission from a damped Ly-α absorber at z = 1.93, and the relation between damped Ly-α absorbers and Lyman-break galaxies.
o	Table 3, text: <[FMW99] SN> (Nos S4-S5), <[FMW99] gA> (Nos gA-gB), <[FMW99] s>, <[FMW99] psf A> (Nos A-B).
Ref:	=2000A&A...358...88F
by	FYNBO J.U. , BURUD I., MOLLER P.
	Astron. Astrophys., 358, 88-94 (2000)
	The sources of extended continuum emission towards Q0151+048A: the host galaxy and the damped Lyα absorber.
o	Table 3: <[FMW99] HGa> (Nos HGa, HGb) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FMZ2005]
[FMZ2005]	(Fan+Ma+Zhou+, 2005)= (Fan)
Write:	<<[FMZ2005] NN>>
N:	62
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	Use of archival Einstein, ROSAT, and Chandra data to search for new X-ray GC candidates in M31.
in source:	M 31 = NGC 224
Ref:	=2005PASP..117.1236F
by	FAN Z. , MA J., ZHOU X., CHEN J., JIANG Z., WU Z.
	Publ. Astron. Soc. Pac., 117, 1236-1249 (2005)
	Identification of X-ray point sources and a study of the nature of 62 X-ray globular cluster candidates in M31.
o	in ref list 1993A&A.272.77B instead of 1993A&AS.272.77B.
o	Table 6: <[FMZ2005] NN> (Nos 1-62).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FN2009]
[FN2009]	(Foster+Nelson, 2009)
Write:	<<[FN2009] NN>>
N:	21
Object:	Void (SIMBAD class: Void = Underdense Region of the Universe)
Note:	N=21 voids in the Updated Zwicky Catalog (UZC).
Ref:	=2009ApJ...699.1252F
by	FOSTER C. , NELSON L.A.
	Astrophys. J., 699, 1252-1260 (2009)
	The size, shape, and orientation of cosmological voids in the Sloan Digital Sky Survey.
o	Table 2: <[FN2009] NN> (Nos 1-21).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FN88]
[FN88]	(Fraix-Burnet+Nieto, 1988) (Not yet in Simbad)
Write:	<<[FN88] Star N>> <<[FN88] Knot HS>> <<[FN88] IntN>> <<[FN88] ExtN>>
N:	7+1+3+6
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Note:	CFHT observations of the jet of 3C 273.
in source:	3C 273
Ref:	=1988A&A...198...87F
by	FRAIX-BURNET D. , NIETO J.-L.
	Astron. Astrophys., 198, 87-99 (1988)
	Quantitative analysis of the optical jet in the QSO 3C 273.
o	A CA Text: <[LNH84] 3C 273 A> (Nos E, F) added. Table 3: <[FN88] Star N> (Nos 1-7). Table 5, Fig.3: <[FN88] Knot HS> N=1, <[FN88] IntN> (Nos Int1 to Int3), <[FN88) ExtN> (Nos Ext1 to Ext6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FNB2011]
[FNB2011]	(Fassbender+Nastasi+Boehringer, 2011)
Write:	<<[FNB2011] N>>
N:	4
Object:	G (SIMBAD class: Galaxy)
Note:	Calar Alto OMEGA2000 and VLT FORS2 observations of the X-ray luminous galaxy cluster XDCP J1007.4+1237. Use of XMM-Newton observations.
in source:	XDCP J1007.0+1237
Ref:	=2011A&A...527L..10F
by	FASSBENDER R. , NASTASI A., BOEHRINGER H., SUHADA R., SANTOS J.S., ROSATI P., PIERINI D., MUEHLEGGER M., QUINTANA H., SCHWOPE A.D., LAMER G., DE HOON A., KOHNERT J., PRATT G.W., MOHR J.J.
	Astron. Astrophys., 527L, 10-10 (2011)
	The X-ray luminous galaxy cluster XMMU J1007.4+1237 at z = 1.56. The dawn of starburst activity in cluster cores.
o	Text: <XDCP J1007.4+1237> N=1. Fig. 1, Table 1: <[FNB2011] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FNB2015]
[FNB2015]	(Fabrizio+Nonino+Bono+, 2015)
Write:	<<[FNB2015] CC NNNNN>>
N:	667
Object:	* (SIMBAD class: Star)
Note:	VLT FLAMES GIRAFFE observations of N=667 stars in the Carina dwarf spheroidal galaxy.
in source:	NAME Carina Dwarf Galaxy
Ref:	=2015A&A...580A..18F
by	FABRIZIO M. , NONINO M., BONO G., PRIMAS F., THEVENIN F., STETSON P.B., CASSISI S., BUONANNO R., COPPOLA G., DA SILVA R.O., DALL'ORA M., FERRARO I., GENOVALI K., GILMOZZI R., IANNICOLA G., MARCONI M., MONELLI M., ROMANIELLO M., WALKER A.R.
	Astron. Astrophys., 580A, 18-18 (2015)
	The Carina Project. VIII. The α-element abundances.
o	Table 2: <[FNB2015] CC NNNNN> N=667 among (Nos 04586-14486).
=E=	Catalogue in electronic form as J/A+A/580/A18
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FNG2002]
[FNG2002]	(Figer+Najarro+Gilmore+, 2002)
Write:	<<[FNG2002] NNN>>
N:	196
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	HST and Keck observations.
in source:	NAME Arches Cluster
Ref:	=2002ApJ...581..258F
by	FIGER D.F. , NAJARRO F., GILMORE D., MORRIS M., KIM S.S., SERABYN E., McLEAN I.S., GILBERT A.M., GRAHAM J.R., LARKIN J.E., LEVENSON N.A., TEPLITZ H.I.
	Astrophys. J., 581, 258-275 (2002)
	Massive stars in the Arches Cluster.
o	Table 3: <[FNG2002] NNN> (Nos 1-196). Table 3: <[LGR2001] ARNN> (Nos AR9-AR17) added.
=E=	Catalogue in electronic form as J/ApJ/581/258
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FNG2005]
[FNG2005]	(Figer+Najarro+Geballe+, 2005)
Write:	<<[FNG2005] NN>>
N:	14
Object:	*inCl (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	UKIRT and Keck observations of stars in the cluster [BDB2003] G010.00-00.24.
in source:	[BDB2003] G010.00-00.24
Ref:	=2005ApJ...622L..49F
by	FIGER D.F. , NAJARRO F., GEBALLE T.R., BLUM R.D., KUDRITZKI R.P.
	Astrophys. J., 622, 49-52 (2005)
	Massive stars in the Sgr 1806-20 cluster.
o	Sgr 1806-20 cluster = [BDB2003] G010.00-00.24
o	Table 1: <[FNG2005] NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FNM2001]
[FNM2001]	(Fuente+Neri+Martin-Pintado+, 2001)
Write:	<<[FNM2001] NGC 7129 MM N>> <<[FNM2001] NGC 7129 FIRS 1 MM N>> <<[FNM2001] NGC 7129 FIRS 2 MM N>> <<[FNM2001] NGC 7129 FIRS 2 IR>>
N:	5+1+2+1
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	IRAM observations.
in source:	NGC 7129
Ref:	=2001A&A...366..873F
by	FUENTE A. , NERI R., MARTIN-PINTADO J., BACHILLER R., RODRIGUEZ-FRANCO A., PALLA F.
	Astron. Astrophys., 366, 873-890 (2001)
	Disks and outflows around intermediate-mass stars and protostars.
o	Table 1, Fig.1: <[FNM2001] NGC 7129 MM N> (Nos 1-5). Table 2, Figs 2, 6: <[FNM2001] NGC 7129 FIRS 1 MM N> (No. 1), <[FNM2001] NGC 7129 FIRS 2 MM N> (Nos 1-2), <[FNM2001] NGC 7129 FIRS 2 IR> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FNO2007]
[FNO2007]	(Fukugita+Nakamura+Okamura+, 2007)
Write:	<<[FNO2007] NNNN>>
N:	2275
Object:	G (SIMBAD class: Galaxy)
Note:	Catalogue of bright galaxies from the SDSS DR3.
Ref:	=2007AJ....134..579F
by	FUKUGITA M. , NAKAMURA O., OKAMURA S., YASUDA N., BARENTINE J.C., BRINKMANN J., GUNN J.E., HARVANEK M., ICHIKAWA T., LUPTON R.H., SCHNEIDER D.P., STRAUSS M.A., YORK D.G.
	Astron. J., 134, 579-593 (2007)
	A catalog of morphologically classified galaxies from the Sloan Digital Sky Survey: north equatorial region.
o	Table 2: <[FNO2007] NNNN> (Nos 1-2275).
=E=	Catalogue in electronic form as J/AJ/134/579
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FNP89]
[FNP89]	(Fraix-Burnet+Nieto+Poulain, 1989)
Write:	<<[FNP89] 3C 66B A>>
N:	5
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Structure of the jet of the rG [N73] 3C 66B: N=5 optical knots (Nos A-E).
in source:	[N73] 3C 66B
Ref:	=1989A&A...221L...1F
by	FRAIX-BURNET D. , NIETO J.-L., POULAIN P.
	Astron. Astrophys., 221, 1-2 (1989)
	Detection of optical polarization in the 3C 66B jet.
o	Fig.1, Table 1: <[FNP89] 3C 66B A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FNS2014]
[FNS2014]	(Fassbender+Nastasi+Santos+, 2014)
Write:	<<[FNS2014] NNa>> <<[FNS2014] aN>> <<[FNS2014] rsN>> <<[FNS2014] s>>
N:	7+3+4+2+1
Object:	G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT HAWK-I, FORS 2 and Subaru SuprimeCam observations of N=7 cluster member galaxies, N=3 cluster member candidates, N=4 foreground galaxies, N=2 "red-locus" galaxies, and N=1 foreground star, in the field of the galaxy cluster XDCP J0044.0-2033.
in source:	XDCP J0044.0-2033
Ref:	=2014A&A...568A...5F
by	FASSBENDER R. , NASTASI A., SANTOS J.S., LIDMAN C., VERDUGO M., KOYAMA Y., ROSATI P., PIERINI D., PADILLA N., ROMEO A.D., MENCI N., BONGIORNO A., CASTELLANO M., CERULO P., FONTANA A., GALAMETZ A., GRAZIAN A., LAMASTRA A., PENTERICCI L., SOMMARIVA V., STRAZZULLO V., SUHADA R., TOZZI P.
	Astron. Astrophys., 568A, 5-5 (2014)
	Galaxy population properties of the massive X-ray luminous galaxy cluster XDCP J0044.0-2033 at z = 1.58 . Red-sequence formation, massive galaxy assembly, and central star formation activity.
o	Fig.17 f,c,s and rs sources not in SIMBAD.
o	Table 1: <[FNS2014] NNa> (Nos 1-2, 3a-3b, 4-6). Fig. 17: <[FNS2014] aN> (Nos c1-c3, f1-f4), <[FNS2014] rsN> (Nos rs1-rs2), <[FNS2014] s> N=1.
=E=	Catalogue in electronic form as <J/A+A/568/A5/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FNS2015]
[FNS2015]	(Feldmeier-Krause+Neumayer+Schoedel+, 2015)
Write:	<<[FNS2015] NNNNN>>
N:	114+705
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT KMOS spectroscopic observations of N=114 bright early-type and N=705 late-type stars in the Galactic Center.
in source:	NAME Gal Center
Ref:	=2015A&A...584A...2F
by	FELDMEIER-KRAUSE A. , NEUMAYER N., SCHOEDEL R., SETH A., HILKER M., DE ZEEUW P.T., KUNTSCHNER H., WALCHER C.J., LUETZGENDORF N., KISSLER-PATIG M.
	Astron. Astrophys., 584A, 2-2 (2015)
	KMOS view of the Galactic centre. I. Young stars are centrally concentrated.
o	Table 2: <[FNS2015] NNNNN> N=29 among (Nos 9-25346). Table 3: <[FNS2015] NNNNN> N=9 among (Nos 88-25347). Tables B1-B3 : <[FNS2015] NNNNN> N=29 among (Nos 64-11652).
Ref:	=2017MNRAS.464..194F
by	FELDMEIER-KRAUSE A. , KERZENDORF W., NEUMAYER N., SCHODEL R., NOGUERAS-LARA F., DO T., DE ZEEUW P.T., KUNTSCHNER H.
	Mon. Not. R. Astron. Soc., 464, 194-209 (2017)
	KMOS view of the Galactic Centre - II. Metallicity distribution of late-type stars.
o	Table B1: <[FNS2015] NNNNN> N=705 among (Nos 1-25496) added.
=E=	Catalogue in electronic form as J/A+A/584/A2
=E=	Catalogue in electronic form as J/MNRAS/464/194
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FNT2004]
[FNT2004]	(Fukugita+Nakamura+Turner+, 2004)
Write:	<<[FNT2004] Galaxy N>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=3 elliptical galaxies with H-alpha emission lines in the SDSS.
Ref:	=2004ApJ...601L.127F
by	FUKUGITA M. , NAKAMURA O., TURNER E.L., HELMBOLDT J., NICHOL R.C.
	Astrophys. J., 601, 127-130 (2004)
	Actively star-forming elliptical galaxies at low redshifts in the Sloan Digital Sky Survey.
o	note 5: galaxy 752-4-8-9449-46 not identified
o	Table 1: <[FNT2004] Galaxy N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FNW2013]
[FNW2013]	(Foyle K.+Natale G.+Wilson+, 2013)
Write:	<<[FNW2013] NN>>
N:	90
Object:	(FIR) (SIMBAD class: FarIR = Far-IR source (λ >= 30 µm))
Note:	N=90 far-infrared compact bright sources detected on the Herschel PACS and SPIRE maps of M83. Use of archival Spitzer IRAC and MIPS data. See also [NFW2014] for a similar work in M33.
Ref:	=2013MNRAS.432.2182F
by	FOYLE K. , NATALE G., WILSON C.D., POPESCU C.C., BAES M., BENDO G.J., BOQUIEN M., BOSELLI A., COORAY A., CORMIER D., DE LOOZE I., FISCHERA J., KARCZEWSKI O.L., LEBOUTEILLER V., MADDEN S., PEREIRA-SANTAELLA M., SMITH M.W.L., SPINOGLIO L., TUFFS R.J.
	Mon. Not. R. Astron. Soc., 432, 2182-2207 (2013)
	Star formation and dust heating in the FIR bright sources of M83.
o	Tables D1-D4: <[FNW2013] NN> (Nos 1-90).
=E=	Catalogue in electronic form as <J/MNRAS/432/2182/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FNW94]
[FNW94]	(Forbes+Norris+Williger+, 1994)
Write:	<<[FNW94] A>> <<[FNW94] East>>
N:	6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 3: Hotspots in NGC 7552, (Nos A-D), No. N (Nucleus) and No. East
in source:	NGC 7552
Ref:	=1994AJ....107..984F
by	FORBES D.A. , NORRIS R.P., WILLIGER G.M., SMITH R.C.
	Astron. J., 107, 984-991 (1994)
	A nuclear starburst ring in the spiral galaxy NGC 7552.
o	Table 3: <[FNW94] A> (Nos A-D, N), <[FNW94] East>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FO
FO	(Forte+Orsatti)
Write:	<<FO NN>>
N:	33
Object:	OB* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Finding charts. OB* in the field of NGC 3372
in source:	NGC 3372 = Carina Nebula
Ref:	=1981AJ.....86..209F
by	FORTE J.C. , ORSATTI A.M.
	Astron. J., 86, 209-216 (1981)
	OB stars in the field of the Carina Nebula.
o	<FO NN> N=33
Origin	of the Acronym: L = Found in the literature
Details on Acronym: FOA
FOA	(Faundez-Oliveira-Abans?)
*****	Avoid the usage of FOA, prefer OA
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FOCA
FOCA	(Focal Objective Corrective Anastigmatism)
Write:	<<FOCA NNNN-NNNN>>
N:	254
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Note:	FOCA balloon experiment. In the format the 4 first digits 'NNNN' stand for: the number of the flight, two first NN, flight No. 07 in ref. 1995A&A...303..661D and an internal number for the plotted direction in the sky, direction No. 28 in ref. 1995A&A...303..661D. The last 4 digits 'NFOCA' stand for an identification number. Table 1: UV sources identified with one G, N=232. Table 2: UV sources identified with two unresolved G
Ref:	=1995A&A...303..661D
by	DONAS J. , MILLIARD B., LAGET M.
	Astron. Astrophys., 303, 661-672 (1995)
	Ultraviolet observations of galaxies in nearby clusters. III. Star-forming galaxies in the Coma cluster.
o	Tables 1, 2: <FOCA 0728-NNNN> N=254 among (Nos 79-2076)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FOCAP
FOCAP	(Fibre Optic Coupled Aperture Plate)= (BFSP) = (SGP)
Write:	<<FOCAP SGPN:NN>> <<FOCAP QSAN:NN>> <<FOCAP QNAN:NN>>
N:	420+824+54
Object:	QSO + * + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	In the format 'AAAN' stands for fields described in Table 3: SGP1 to 7, QSF1 to 5, QNB1 to 2, QNY1 to 5, QNA1, QNZ1 to 5, QSM1 to 8, QSI2 and 4.
Ref:	=1990MNRAS.243....1B
by	BOYLE B.J. , FONG R., SHANKS T., PETERSON B.A.
	Mon. Not. R. Astron. Soc., 243, 1-56 (1990)
	A catalogue of faint, UV-excess objects.
o	Tables 6, 7, 8: <FOCAP AAAN:NN>, N=522+824+54
=E=	Catalogue in electronic form as J/MNRAS/243/1
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FOCAS
FOCAS	(Faint Object Classif. and Analysis System)
*****	Avoid the usage of FOCAS, prefer [WBD96]
Origin	of the Acronym: L (1998A&AS..129..583F)
Details on Acronym: [FOK2018]
[FOK2018]	(Fujimoto+Ouchi+Kohno+, 2018)= (ASAGAO)
Write:	<<[FOK2018] NNN>>
N:	42
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	ALMA band 6 observations of N=42 sources in the GOODS South field, as part of the Alma twenty-Six Arcmin² survey of GOODS-South At One-millimeter (ASAGAO).
in source:	NAME GOODS South Field
Ref:	=2018ApJ...861....7F
by	FUJIMOTO S. , OUCHI M., KOHNO K., YAMAGUCHI Y., HATSUKADE B., UEDA Y., SHIBUYA T., INOUE S., OOGI T., TOFT S., GOMEZ-GUIJARRO C., WANG T., ESPADA D., NAGAO T., TANAKA I., AO Y., UMEHATA H., TANIGUCHI Y., NAKANISHI K., RUJOPAKARN W., IVISON R.J., WANG W.-H., LEE M.M., TADAKI K.-I., TAMURA Y., DUNLOP J.S.
	Astrophys. J., 861, 7-7 (2018)
	ALMA 26 arcmin^{2} survey of GOODS-S at one millimeter (ASAGAO): average morphology of high-z dusty star-forming galaxies in an exponential disk (n ≃ 1).
o	Table 1: <[FOK2018] NNN> N=42 among (Nos 1-613).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FOO2016]
[FOO2016]	(Fujimoto+Ouchi+Ono+, 2016)
Write:	<<[FOO2016] NNN>> <<[FOO2016] ANN>> <<[FOO2016] IDNNN>> (not recognised by Simbad, but found in literature)
N:	133+18
Object:	(mm) + (Opt) + (NIR) + Poss. Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=133 faint 1.2mm continuum sources detected in deep ALMA Band 6 observations. N=15+2 optical-NIR counterparts. N=1 very strongly lensed source candidate.
Ref:	=2016ApJS..222....1F
by	FUJIMOTO S. , OUCHI M., ONO Y., SHIBUYA T., ISHIGAKI M., NAGAI H., MOMOSE R.
	Astrophys. J., Suppl. Ser., 222, 1 (2016)
	ALMA census of faint 1.2 mm sources down to ~ 0.02 mJy: extragalactic background light and dust-poor, high-z galaxies.
o	Table 3: <[FOO2016] NNN> (Nos 1-133). Tables 7+10: <[FOO2016] ANN> (Nos S1-S15, A1-A2). Fig. 11, Table 9: <[FOO2016] AN> (No. A3).
=E=	Catalogue in electronic form as <J/ApJS/222/1/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FOP2009]
[FOP2009]	(Fiolet+Omont+Polletta+, 2009)
Write:	<<[FOP2009] L-NN>>
N:	33
Object:	Submm G (SIMBAD class: Galaxy)
Note:	Mayall 4m telescope MOSAIC, Palomar WIRC, and UKIRT WFCAM observations of N=33 z∼2 SMG candidates, in a field part of the SWIRE Lockman Hole field. Use of SWIRE data.
Ref:	=2009A&A...508..117F
by	FIOLET N. , OMONT A., POLLETTA M., OWEN F., BERTA S., SHUPE D., SIANA B., LONSDALE C., STRAZZULLO V., PANNELLA M., BAKER A.J., BEELEN A., BIGGS A., DE BREUCK C., FARRAH D., IVISON R., LAGACHE G., LUTZ D., TACCONI L.J., ZYLKA R.
	Astron. Astrophys., 508, 117-132 (2009)
	Multi-wavelength properties of Spitzer selected starbursts at z~2.
o	Table 1: <[FOP2009] L-NN> (Nos L-1 to L-33).
o	Fig.9 IRAS 20551-4850 is a probable misprint for IRAS 20551-4250.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FOP2010]
[FOP2010]	(Fumagalli+O'Meara+Prochaska+, 2010) (Not yet in Simbad)
Write:	<<[FOP2010] QSO JHHMMSS+DDMMSS A>>
N:	18+12
Object:	G (SIMBAD class: Galaxy)
Note:	Keck I LRIS observations of possible host galaxies of damped Lymanα absorbers.
Ref:	=2010MNRAS.408..362F
by	FUMAGALLI M. , O'MEARA J.M., PROCHASKA J.X., KANEKAR N.
	Mon. Not. R. Astron. Soc., 408, 362-382 (2010)
	Directly imaging damped Lyman α galaxies at z>2 - I. Methodology and first results.
o	Fig. 2, Table 3: <[FOP2010] QSO JHHMMSS+DDMMSS A> N=18+12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FOP2011]
[FOP2011]	(Fumagalli+O'Meara+Prochaska, 2011)
Write:	<<[FOP2011] LLS1134a>> <<[FOP2011] LLS0956A>>
N:	2+2
Object:	LLS
Note:	Keck I HIRES observations of N=2+2 Lyman limit systems in the line of sight of the observed quasars SDSS J113418.96+574204.6 and QSO B0956+122.
Ref:	=2011Sci...334.1245F
by	FUMAGALLI M. , O'MEARA J.M., PROCHASKA J.X.
	Sci, 334, 1245-1249 (2011)
	Detection of pristine gas two billion years after the Big Bang.
o	<[FOP2011] LLS1134a> (Nos LLS1134a-LLS1134b), <[FOP2011] LLS0956A> (Nos LLS0956A-LLS0956B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ford
Ford	(Ford+)= (CJFN) = (F) = ([FJ78]) = (P)
Write:	<<Ford M 31 NNN>>
N:	742
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	(Nos 138, 188, 192, 262, 524, 543) missing. See also: [JCF89], [CJF89], [JCF90], [CJH91], [MCJ93], [JCH96], [FCJ97], [CJF98]
in source:	M 31 = NGC 224
Ref:	=1978ApJS...38..351F
by	FORD H.C. , JACOBY G.H.
	Astrophys. J., Suppl. Ser., 38, 351-356 (1978)
	Planetary nebulae in local-group galaxies. VIII. A catalog of planetary nebulae in the Andromeda galaxy.
o	Table 2: <Ford M 31 NNN> N=311 among (Nos 1-315)
Ref:	=1982ApJ...256..120L
by	LAWRIE D.G. , FORD H.C.
	Astrophys. J., 256, 120-126 (1982)
	Planetary nebulae in Local Group galaxies. IX. Velocity modulated photographs of the center of M 31.
o	Table 3 not in SIMBAD
o	Table 2: <Ford M 31 NNN> (Nos 316-334). Table 3: [LF82] a> (Nos a-d).
Ref:	=1987ApJ...317...62N
by	NOLTHENIUS R. , FORD H.C.
	Astrophys. J., 317, 62-81 (1987)
	Dynamics of the outer disk and halo of M 31.
o	Table 3: <Ford M 31 NNN> (Nos 335-371).
Ref:	=1989ApJ...339...53C
by	CIARDULLO R. , JACOBY G.H., FORD H.C., NEILL J.D.
	Astrophys. J., 339, 53-69 (1989)
	Planetary nebulae as standard candles. II. The calibration in M 31 and its companions.
o	Table 2: <Ford M 31 NNN> (Nos 372-569), Table 6: <Ford NGC 185 N> No. 5 , <Ford NGC 205 NN> N=12 among (Nos 13-28), <Ford NGC 205 a> N=9 among (Nos a-k), <Ford NGC 221 NN> (Nos 29-30)
Ref:	=2002ApJ...577...31C
by	CIARDULLO R. , FELDMEIER J.J., JACOBY G.H., KUZIO DE NARAY R., LAYCHAK M.B., DURRELL P.R.
	Astrophys. J., 577, 31-50 (2002)
	Planetary nebulae as standard candles. XII. Connecting the population I and population II distance scales.
o	Table 2: <Ford M 31 NNN> (Nos 570-742) added. Table 3: <[CFJ2002] NGC 2403 NN> (Nos 1-40). Table 4: <[CFJ2002] NGC 3115 NN> (Nos 1-62). Table 5: <[CFJ2002] NGC 3351 NN> (Nos 1-20). Table 6: <[CFJ2002] NGC 3627 NN> (Nos 1-73). Table 7: <[CFJ2002] NGC 4258 NN> (Nos 1-58). Table 8: <[CFJ2002] NGC 5866 NN> (Nos 1-24).
=E=	Catalogue in electronic form as J/ApJ/339/53
=E=	Catalogue in electronic form as J/ApJ/577/31
=E=	Catalogue in electronic form as J/ApJS/38/351
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ford
Ford	(Ford+)
Write:	<<Ford NGC 185 N>> <<Ford NGC 205 NN>> <<Ford NGC 205 a>> <<Ford NGC 221 NN>> <<Ford NGC 221 a>>
N:	79
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	see also FJJ
in source:	NGC 185
in source:	NGC 205 = M 110
in source:	NGC 221 = M 32
Ref:	=1973ApJ...183L..73F
by	FORD H.C. , JENNER D.C., EPPS H.W.
	Astrophys. J., 183, 73-75 (1973)
	Planetary nebulae in Local Group galaxies. I. Identifications in NGC 185, NGC 205, and NGC 221.
o	<Ford NGC 185 N> (Nos 1-4), <Ford NGC 205 NN> (Nos 1-12), <Ford NGC 221 NN> (Nos 1-12)
Ref:	=1975ApJ...202..365F
by	FORD H.C. , JENNER D.C.
	Astrophys. J., 202, 365-371 (1975)
	Planetary nebulae in Local Group galaxies. II. Identifications, positions, number, and production rate of nebulae in NGC 221.
o	Table 2: <Ford NGC 221 NN> (Nos 13-22), Table 3: <Ford NGC 221 a> N=7 among (Nos a-m)
Ref:	=1983IAUS..103..443F
by	FORD H.C.
	IAU Symp., 103, held at University College, London, U.K. August 9-13, 1982 Ed. by D.R. Flower., 103, 443-460 (1983)
	Planetary nebulae in local goup galaxies.
o	Fig. 1: <Ford NGC 221 NN> (Nos 23-28)
Ref:	=1989ApJ...339...53C
by	CIARDULLO R. , JACOBY G.H., FORD H.C., NEILL J.D.
	Astrophys. J., 339, 53-69 (1989)
	Planetary nebulae as standard candles. II. The calibration in M 31 and its companions.
o	Table 2: <Ford M 31 NNN> (Nos 372-569), Table 6: <Ford NGC 185 N> No. 5 , <Ford NGC 205 NN> N=12 among (Nos 13-28), <Ford NGC 205 a> N=9 among (Nos a-k), <Ford NGC 221 NN> (Nos 29-30)
=E=	Catalogue in electronic form as J/ApJ/339/53
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Fornax
Fornax	(Fornax region)= (H)
Write:	<<NAME Fornax N>>
N:	6
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Rem:	Identif. charts
in source:	NAME Fornax Dwarf Galaxy
Ref:	=1961AJ.....66...83H
by	HODGE P.W.
	Astron. J., 66, 83-84 (1961)
	The Fornax dwarf galaxy. I. The globulars clusters.
o	<NAME Fornax N> (Nos 1-5) = <NAME Fornax HN> (Nos H1-H5).
Ref:	=1969PASP...81..875H
by	HODGE P.W.
	Publ. Astron. Soc. Pac., 81, 875-878 (1969)
	The color indices of the globular clusters of the Fornax dwarf galaxy.
o	<NAME FORNAX N> (No. 6) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FOS2017]
[FOS2017]	(Fujimoto+Ouchi+Shibuya+, 2017)
Write:	<<[FOS2017] NNNN>>
N:	1034
Object:	G (SIMBAD class: Galaxy)
Note:	Detection of N=1034 submm/mm continuum sources in ALMA band 6/7 observations. Use of archival ALMA data.
Ref:	=2017ApJ...850...83F
by	FUJIMOTO S. , OUCHI M., SHIBUYA T., NAGAI H.
	Astrophys. J., 850, 83-83 (2017)
	Demonstrating A New Census of INfrared Galaxies with ALMA (DANCING-ALMA). I. FIR size and luminosity relation at z = 0-6 revealed with 1034 ALMA sources.
o	Table 4: <[FOS2017] NNNN> (Nos 1-1034).
=E=	Catalogue in electronic form as J/ApJ/850/83
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FOV
FOV	(FIRST Optical VLA)
Write:	<<FOV JHHMM+DDMM>> <<FOV JHHMM+DDMM W>>
N:	92+5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Identification of radio lobes in FIRST images. VLA 6cm observations of these sources. See also [HWF2005]
Ref:	=2005AJ....130.1977H
by	HAARSMA D.B. , WINN J.N., FALCO E.E., KOCHANEK C.S., AMMAR P., BOERSMA C., FOGWELL S., MUXLOW T.W.B., McLEOD B.A., LEHAR J.
	Astron. J., 130, 1977-1995 (2005)
	The FIRST-Optical-VLA survey for lensed radio lobes.
o	Table 1: <FOV JHHMM+DDMM> N=92. Table 2: <FOV JHHMM+DDMM W> N=5. Table 2, cols(2, 3): <[HWF2005] JHHMMSS.ss+DDMMSS.s> N=32.
=E=	Catalogue in electronic form as J/AJ/130/1977
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FOW2011]
[FOW2011]	(Forbrich+Osten+Wolk, 2011)
Write:	<<[FOW2011] NN>>
N:	26
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 3.6cm and 6cm observations of the fields of IC 348 and NGC 1333.
in source:	IC 348
in source:	NGC 1333
Ref:	=2011ApJ...736...25F
by	FORBRICH J. , OSTEN R.A., WOLK S.J.
	Astrophys. J., 736, 25 (2011)
	Simultaneous X-ray and radio observations of young stellar objects in NGC 1333 and IC 348.
o	Tables 2+6: <[FOW2011] NN> (Nos 1-26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FP
FP	(Frew+Parker)
Write:	<<FP JHHMM+DDMM>>
N:	13
Object:	Poss. PN (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
Note:	MASH (Macquarie-AAO-Strasbourg H-alpha) catalog. MASH-II: 2008MNRAS.384..525M. Search for PNe in the SuperCOSMOS Halpha survey. See also PN, PHR, PPA.
Ref:	=2006MNRAS.373...79P
by	PARKER Q.A. , ACKER A., FREW D.J., HARTLEY M., PEYAUD A.E.J., OCHSENBEIN F., PHILLIPPS S., RUSSEIL D., BEAULIEU S.F., COHEN M., KOEPPEN J., MISZALSKI B., MORGAN D.H., MORRIS R.A.H., PIERCE M.J., VAUGHAN A.E.
	Mon. Not. R. Astron. Soc., 373, 79-94 (2006)
	The Macquarie/AAO/Strasbourg Hα Planetary Nebula Catalogue: MASH.
o	Catalogue: <PHR JHHMM+DDMM> N=749. Catalogue: <FP JHHMM+DDMM> N=13. Catalogue: <PPA JHHMM+DDMM> N=137. <NAME HP JHHMM+DDMM> N=1. <NAME PKP JHHMM+DDMM> N=2.
=E=	Catalogue in electronic form as V/127
=E=	Catalogue in electronic form as <V/127A/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FP2004]
[FP2004]	(Ferreiro+Pastoriza, 2004)
Write:	<<[FP2004] AM HHMM+DDdWW>> <<[FP2004] AM HHMM+DDdWW NN>> <<[FP2004] AM HHMM+DDdWW A>> <<[FP2004] AM HHMM+DDdWW a>>
N:	22+118
Object:	G in Pair + HII (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	CTIO 0.9m telescope photometry of 11 pair of AM galaxies. The 2 components (main and secondary) are noted by their direction 'WW'. HII regions in each components are found.
in source:	AM 1256-433
in source:	AM 1401-324
in source:	AM 1448-262
in source:	AM 2030-303
in source:	AM 2058-381
in source:	AM 2105-332
in source:	AM 2229-735
in source:	AM 2238-575
in source:	AM 2306-721
in source:	AM 2322-821
in source:	AM 2330-451
Ref:	=2004A&A...428..837F
by	FERREIRO D.L. , PASTORIZA M.G.
	Astron. Astrophys., 428, 837-846 (2004)
	Sample of minor merger of galaxies: Optical CCD surface photometry and HII region properties.
o	Table 4: <[FP2004] AM HHMM+DDdWW> N=22. Table 5: <[FP2004] AM HHMM+DDdWW NN>, <[FP2004] AM HHMM+DDdWW A>, <[FP2004] AM HHMM+DDdWW a>, N=118.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FP2007]
[FP2007]	(Forbrich+Preibisch, 2007)
Write:	<<[FP2007] JHHMMSS.ss+DDMMSS.s>>
N:	92
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of the Coronet Cluster.
in source:	Coronet Cluster = R CRa Cluster
Ref:	=2007A&A...475..959F
by	FORBRICH J. , PREIBISCH T.
	Astron. Astrophys., 475, 959-972 (2007)
	Coronae in the Coronet: a very deep X-ray look into a stellar nursery.
o	Table a1: <[FP2007] JHHMMSS.ss+DDMMSS.s> N=92.
=E=	Catalogue in electronic form as <J/A+A/475/959/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FP74]
[FP74]	(Frogel+Persson, 1974)= (IRS)
Write:	<<[FP74] RCW NN IRS N>> <<[FP74] W 22 IRS N>>
N:	3+5+3+1+1
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	IRS in 5 HII regions. See also [FPA77].
in source:	RCW 38
in source:	RCW 57
in source:	RCW 97
in source:	RCW 49
in source:	W 22
Ref:	=1974ApJ...192..351F
by	FROGEL J.A. , PERSSON S.E.
	Astrophys. J., 192, 351-368 (1974)
	Compact infrared sources associated with southern H II regions.
o	T.1: HII regions are [GS70] LLL.l+B.b (Numbering 'NN' not used).
o	Fig.2: <[FP74] RCW 38 IRS N> (Nos 1-3). Fig.5: <[FP74] RCW 57 IRS N> (Nos 1-5). Fig.8: <[FP74] RCW 97 IRS N> (Nos 1-3). Fig.9: <[FP74] RCW 49 IRS N> (No.1). Fig.10: <[FP74] W 22 IRS N> (No.1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPA2009]
[FPA2009]	(Fernandez-Ontiveros+Prieto+Acosta-Pulido, 2009) (Not yet in Simbad)
Write:	<<[FPA2009] NN>>
N:	7
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	VLT NACO AO and VISIR observations of infrared bright knots in the central 300pc of NGC 253.
in source:	NGC 253
Ref:	=2009MNRAS.392L..16F
by	FERNANDEZ-ONTIVEROS J.A. , PRIETO M.A., ACOSTA-PULIDO J.A.
	Mon. Not. R. Astron. Soc., 392L, 16-20 (2009)
	The nucleus of NGC 253 and its massive stellar clusters at parsec scales.
o	Figs 1-2, Table 1: <[FPA2009] NN> N=7 among (Nos 4-35).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPA2012]
[FPA2012]	(Frey+Paragi+An+, 2012)
Write:	<<[FPA2012] WW>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLBI observations of N=2 radio components in the quasar SDSS J142507.32+323137.4.
in source:	QSO J1425+3231
Ref:	=2012MNRAS.425.1185F
by	FREY S. , PARAGI Z., AN T., GABANYI K.E.
	Mon. Not. R. Astron. Soc., 425, 1185-1191 (2012)
	Two in one? a possible dual radio-emitting nucleus in the quasar SDSS J1425+3231.
o	<[FPA2012] WW> (Nos NW, SE).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPA77]
[FPA77]	(Frogel+Persson+Aaronson, 1977)= (IRS)
Write:	<<[FPA77] GLLL.l+B.b IRS N>> <<[FPA77] NGC 3603 IRS NNA>>
N:	7+12+3+1
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Las Campanas observations. IRS in HII regions. See also [FP74].
in source:	GAL 291.6-00.5
in source:	GAL 333.1-00.4
in source:	GAL 337.9-00.5
in source:	GAL 348.2-01.0
in source:	GAL 348.7-01.0
in source:	NGC 3603
Ref:	=1977ApJ...213..723F
by	FROGEL J.A. , PERSSON S.E., AARONSON M.
	Astrophys. J., 213, 723-736 (1977)
	Compact infrared sources associated with southern HII regions. II.
o	Table 2: <[FPA77] GLLL.l+B.b IRS N> N=7. Table 3: <[FPA77] NGC 3603 IRS NN> N=12 among (Nos 1-15).
Ref:	=2003A&A...400..223N
by	NUERNBERGER D.E.A. , STANKE T.
	Astron. Astrophys., 400, 223-239 (2003)
	Infrared observations of NGC3603. II. A 11.9µm and 18µm survey.
o	Fig.2: Shock Front SF 1 to SF 7 not in SIMBAD. Table 2: Sher 25 = NGC 3603 25, Stars MTT AN are CL* NGC 3603 BLW AN in SIMBAD.
o	Table 2: <[NS2003] NNA> N=77, (Nos 1-48). Table 2: <[FPA77] NGC 3603 IRS NNA> (Nos 9A-9C) added.
Ref:	=2008RMxAC..33..145N
by	NURNBERGER D.E.A.
	RMxAC, 33, 145-147 (2008)
	Exciting new vistas on the formation of high mass stars.
o	Fig. 2: <[FPA77] NGC 3603 NNA> (No. 9D added), <[N2008] NGC 3603 NA-N> (Nos 9A-1 to 9A-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPB2012]
[FPB2012]	(fontani+Palau+Busquet+, 2012)
Write:	<<[FPB2012] MMA>> <<[FPB2012] IRS3-SW>>
N:	5+1
Object:	mm Condensation + Cloud (SIMBAD class: denseCore = Dense Core)
Note:	CARMA (3mm) and VLA (1.3cm and NH3) observations of N=5 mm continuum condensations in the star-forming region IRAS 20343+4129 and N=1 cloud south-west of [KBD2002] IRAS 20343+4129 IRS 3.
in source:	IRAS 20343+4129
Ref:	=2012MNRAS.423.1691F
by	FONTANI F. , PALAU A., BUSQUET G., ISELLA A., ESTALELLA R., SANCHEZ-MONGE A., CASELLI P., ZHANG Q.
	Mon. Not. R. Astron. Soc., 423, 1691-1706 (2012)
	Dense gas in IRAS 20343+4129: an ultracompact H II region caught in the act of creating a cavity.
o	Fig. 2, Table 3: <[FPB2012] MMA> (Nos MMA-MME). Fig. 3: <[FPB2012] IRS3-SW> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPB97]
[FPB97]	(Fender+Pooley+Brocksopp+, 1997)
Write:	<<[FPB97] Star A>>
N:	2
Object:	* (SIMBAD class: Star)
Note:	Fig.1: N=2 stars in the field of Granat 1915+105. Finding chart, no coordinates.
Ref:	=1997MNRAS.290L..65F
by	FENDER R.P. , POOLEY G.G., BROCKSOPP C., NEWELL S.J.
	Mon. Not. R. Astron. Soc., 290, 65-69 (1997)
	Rapid infrared flares in GRS 1915+105: evidence for infrared synchrotron emission.
o	Fig.1: <[FPB97] Star A> (Nos A-B)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPC2000]
[FPC2000]	(Fasano+Poggianti+Couch+, 2000)
Write:	<<[FPC2000] ACO NNNN NN>>
N:	393
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	ACO 3330
in source:	ACO 389
in source:	ACO 951
in source:	ACO 2658
in source:	ACO 2192
in source:	ACO 1643
in source:	ACO 2111
in source:	ACO 1952
in source:	ACO 1878
Ref:	=2000ApJ...542..673F
by	FASANO G. , POGGIANTI B.M., COUCH W.J., BETTONI D., KJAERGAARD P., MOLES M.
	Astrophys. J., 542, 673-683 (2000)
	The evolution of the galactic morphological types in clusters.
o	Right ascensions are 8" too far East in ACO 1643.
o	Table 3: <[FPC2000] ACO 3330 NN> (Nos 1-47), <[FPC2000] ACO 389 NN> (Nos 1-38), <[FPC2000] ACO 951 NN> (Nos 1-24), <[FPC2000] ACO 2658 NN> (Nos 1-20), <[FPC2000] ACO 2192 NN> (Nos 1-49), <[FPC2000] ACO 1643 NN> (Nos 1-47), <[FPC2000] ACO 2111 NN> (Nos 1-67), <[FPC2000] ACO 1952 NN> (Nos 1-53), <[FPC2000] ACO 1878 NN> (Nos 1-38).
=E=	Catalogue in electronic form as J/ApJ/542/673
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPC2010]
[FPC2010]	(Fleener+Payne+Chu+, 2010)
Write:	<<[FPC2010] JHHMMSS.ss+DDMMSS.s>>
N:	10
Object:	Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 and CTIO 4m Blanco telescope ISPI observations of NGC 2074.
in source:	NGC 2074
Ref:	=2010AJ....139..158F
by	FLEENER C.E. , PAYNE J.T., CHU Y.-H., CHEN C.-H.R., GRUENDL R.A.
	Astron. J., 139, 158-167 (2010)
	Massive star formation in NGC 2074.
o	Table 1: <[FPC2010] JHHMMSS.ss+DDMMSS.s> N=10.
Details on Acronym: [FPC2011]
[FPC2011]	(Fontani+Palau+Caselli+, 2011)
Write:	<<[FPC2011] I22134-A>> <<[FPC2011] I22134-VLA1>>
N:	2+1
Object:	Core (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	IRAM 30m N2H+ and N2D+ observation of dense cores in the field of IRAS 22134+5834.
Ref:	=2011A&A...529L...7F
by	FONTANI F. , PALAU A., CASELLI P., SANCHEZ-MONGE A., BUTLER M.J., TAN J.C., JIMENEZ-SERRA I., BUSQUET G., LEURINI S., AUDARD M.
	Astron. Astrophys., 529L, 7-7 (2011)
	Deuteration as an evolutionary tracer in massive-star formation.
o	(Erratum) + corrigendum vol. 562, p. C1 (2014)
o	Table A.1: <[FPC2011] I22134-A> (Nos B, G), <[FPC2011] I22134-VLA1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPC2014]
[FPC2014]
Write:	<<[FPC2014] NNNNNNN>>
N:	44811
Object:	* (SIMBAD class: Star)
Note:	MDM Observatory 2.4m Hiltner telescope BVI photometry of N=44811 stars in the globular cluster M15.
in source:	M 15 = NGC 7078
Ref:	=2014PASP..126..733F
by	FEUILLET D.K. , PAUST N.E.Q., CHABOYER B.
	PASP, 126, 733-738 (2014)
	BVI photometry and the red giant branch luminosity function of M 15.
o	Table 1: <[FPC2014] NNNNNNN> N=44811 among (Nos 2-5050990).
=E=	Catalogue in electronic form as J/PASP/126/733
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPC2015]
[FPC2015]	(Falocco+Paolillo+Covone+, 2015)
Write:	<<[FPC2015] NNNNNN>>
N:	175
Object:	* + AGN + SN + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=175 AGN candidates selected from the SUDARE-VOICE survey performed with the VLT Survey Telescope (VST). See also [DPC2015].
in source:	NAME CDFS
Ref:	=2015A&A...579A.115F
by	FALOCCO S. , PAOLILLO M., COVONE G., DE CICCO D., LONGO G., GRADO A., LIMATOLA L., VACCARI M., BOTTICELLA M.T., PIGNATA G., CAPPELLARO E., TREVESE D., VAGNETTI F., SALVATO M., RADOVICH M., HSU L., CAPACCIOLI M., NAPOLITANO N., BRANDT W.N., BARUFFOLO A., CASCONE E., SCHIPANI P.
	Astron. Astrophys., 579A, 115-115 (2015)
	SUDARE-VOICE variability-selection of active galaxies in the Chandra Deep Field-South and the SERVS/SWIRE region.
o	Table 3: <[FPC2015] NNNNNN> N=175 among (Nos 290-110606).
=E=	Catalogue in electronic form as <J/A+A/579/A115/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPD2001]
[FPD2001]	(Ferraro+Possenti+D'Amico+, 2001)= ([FPD2001a])
Write:	<<[FPD2001] A>>
N:	3
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	HST observations. N=3 stars in the error box of PSR J1740-5340.
Ref:	=2001ApJ...561L..93F
by	FERRARO F.R. , POSSENTI A., D'AMICO N., SABBI E.
	Astrophys. J., 561, 93-96 (2001)
	The bright optical companion to the eclipsing millisecond pulsar in NGC 6397.
o	Fig.1: <[FPD2001] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPD2001a]
[FPD2001a]	(Ferraro+Possenti+D'Amico+, 2001)
*****	Avoid the usage of [FPD2001a], prefer [FPD2001]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPD2001b]
[FPD2001b]	(Fanti+Pozzi+Dallacasa+, 2002)
Write:	<<[FPD2001b] HHMM+DDdA N>>
N:	226+46
Object:	Component (SIMBAD class: Radio = Radio Source)
Note:	Radio components of 87 B3 sources. See also [DTF2002], [DFG2002].
Ref:	=2001A&A...369..380F
by	FANTI C. , POZZI F., DALLACASA D., FANTI R., GREGORINI L., STANGHELLINI C., VIGOTTI M.
	Astron. Astrophys., 369, 380-420 (2001)
	Multi-frequency VLA observations of a new sample of CSS/GPS radio sources.
o	Tables 3, 3b: <[FPD2001b] HHMM+DDdA N> N=226+46.
=E=	Catalogue in electronic form as J/A+A/369/380
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPD2013]
[FPD2013]	(Finkelstein+Papovich+Dickinson+, 2013)
Write:	<<[FPD2013] z8 GND 5296>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Note:	Keck I MOSFIRE NIR spectroscopy of N=1 galaxy in the GOODS-North Deep Field.
in source:	NAME GOODS North Field
Ref:	=2013Natur.502..524F
by	FINKELSTEIN S.L. , PAPOVICH C., DICKINSON M., SONG M., TILVI V., KOEKEMOER A.M., FINKELSTEIN K.D., MOBASHER B., FERGUSON H.C., GIAVALISCO M., REDDY N., ASHBY M.L.N., DEKEL A., FAZIO G.G., FONTANA A., GROGIN N.A., HUANG J.-S., KOCEVSKI D., RAFELSKI M., WEINER B.J., WILLNER S.P.
	Natur, 502, 524-527 (2013)
	A galaxy rapidly forming stars 700 million years after the Big Bang at redshift 7.51.
o	<[FPD2013] z8 GND 5296> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPE2007]
[FPE2007]	(Feain+Papadopoulos+Ekers+, 2007)
Write:	<<[FPE2007] CN>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA 6.2GHz and 8.4GHz continuum observations of HE 0450-2958.
in source:	HE 0450-2958
Ref:	=2007ApJ...662..872F
by	FEAIN I.J. , PAPADOPOULOS P.P., EKERS R.D., MIDDELBERG E.
	Astrophys. J., 662, 872-877 (2007)
	Dressing a naked quasar: star formation and active galactic nucleus feedback in HE 0450-2958.
o	Fig.1, Table 2: <[FPE2007] CN> (Nos C1-C3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPF2021]
[FPF2021]	(Fritz+Patrick+Feldmeier-Krause+, 2021)
Write:	<<[FPF2021] NNN NN N>>
N:	3065
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	ESO VLT KMOS observations of N=3065 stars in the nuclear disk of the Milky Way.
Ref:	=2021A&A...649A..83F
by	FRITZ T.K. , PATRICK L.R., FELDMEIER-KRAUSE A., SCHODEL R., SCHULTHEIS M., GERHARD O., NANDAKUMAR G., NEUMAYER N., NOGUERAS-LARA F., PRIETO M.A.
	Astron. Astrophys., 649A, 83-83 (2021)
	A KMOS survey of the nuclear disk of the Milky Way. I. Survey design and metallicities.
o	Table E1: <[FPF2021] NNN NN N> N=3065.
=E=	Catalogue in electronic form as <J/A+A/649/A83/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPG2010]
[FPG2010]	(Finkelstein+Papovich+Giavalisco+, 2010)
Write:	<<[FPG2010] NNNN>>
N:	31
Object:	G (SIMBAD class: Galaxy)
Note:	HST WFC3 observations of the HUDF.
in source:	NAME HUDF
Ref:	=2010ApJ...719.1250F
by	FINKELSTEIN S.L. , PAPOVICH C., GIAVALISCO M., REDDY N.A., FERGUSON H.C., KOEKEMOER A.M., DICKINSON M.
	Astrophys. J., 719, 1250-1273 (2010)
	On the stellar populations and evolution of star-forming galaxies at 6.3 < z ≤ 8.6.
o	Table 1: <[FPG2010] NNNN> N=31 among (Nos 125-3053).
Details on Acronym: [FPG2012]
[FPG2012]	(Fiore+Puccetti+Grazian+, 2012)
Write:	<<[FPG2012] ENNNNN>> <<[FPG2012] MNNNNN>> <<[FPG2012] 216554>>
N:	21+43+1 (SIMBAD class: Galaxy)
Note:	Chandra observations of GOODS-ERS and GOODS-MUSIC z > 3 galaxies.
Ref:	=2012A&A...537A..16F
by	FIORE F. , PUCCETTI S., GRAZIAN A., MENCI N., SHANKAR F., SANTINI P., PICONCELLI E., KOEKEMOER A.M., FONTANA A., BOUTSIA K., CASTELLANO M., LAMASTRA A., MALACARIA C., FERUGLIO C., MATHUR S., MILLER N., PANNELLA M.
	Astron. Astrophys., 537A, 16-16 (2012)
	Faint high-redshift AGN in the Chandra Deep Field South: the evolution of the AGN luminosity function and black hole demography.
o	Tables 1,2 : <[FPG2012] ENNNNN> N=21 among (Nos E537-E10247), <[FPG2012] MNNNNN> N=44 among (Nos M208-M70531), <[FPG2012] 216554> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPG93]
[FPG93]	(Folgheraitre+Penny+Griffiths, 1993)
Write:	<<[FPG93] NN>>
N:	50
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	NGC 6205 = M 13
Ref:	=1993MNRAS.264..991F
by	FOLGHERAITER E.L. , PENNY A.J., GRIFFITHS W.K.
	Mon. Not. R. Astron. Soc., 264, 991-998 (1993)
	The chemical inhomogenity of M 13.
o	<[FPG93] NN> N=50
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPG99]
[FPG99]	(Feretti+Perley+Giovannini+, 1999)
Write:	<<[FPG99] 3C 449 WN>> <<[FPG99] HHMMSS.s+DDMMSS.s>>
N:	2+9+1
Object:	Radio component (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	3C 449 present 2 opposite jets North and South, with knots in each jet. An extended unrelated source '222836.5+390847.7' is observed in the field of 3C 449.
in source:	3C 449
Ref:	=1999A&A...341...29F
by	FERETTI L. , PERLEY R., GIOVANNINI G., ANDERNACH H.
	Astron. Astrophys., 341, 29-None (1999)
	VLA observations of the giant radio galaxy 3C 449.
o	Fig.1: <[FPG99] 3C 449 WN> (Nos N, S, S1-S4, N1-N5). p.31: <[FPG99] HHMMSS.s+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPH98]
[FPH98]	(Filipovic+Pietsch+Haynes+, 1998)
Write:	<<[FPH98] LMC NN>> <<[FPH98] SMC NN>>
N:	71+27
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 2, col(1): (Nos 1-71), catalogue of LMC radio-sources identified in the ROSAT All-Sky Survey. cross-id col(2): [FHW95]. cross-id col(3): LMC RASS. Table 3, col(1): (Nos 1-27), catalogue of SMC radio-sources identified in the ROSAT PSPC. cross-id col(2): [FJW97]. cross-id col(3): RX
in source:	Magellanic Clouds:LMC = LMC
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1998A&AS..127..119F
by	FILIPOVIC M.D. , PIETSCH W., HAYNES R.F., WHITE G.L., JONES P.A., WIELEBINSKI R., KLEIN U., DENNERL K., KAHABKA P., LAZENDIC J.S.
	Astron. Astrophys., Suppl. Ser., 127, 119-138 (1998)
	A radio continuum study of the Magellanic Clouds. VI. Discrete sources common to radio and X-ray surveys of the Magellanic Clouds.
o	Table 2, col(1): <[FPH98] LMC NN> (Nos 1-71). Table 2, col(3): <LMC RASS NNNN> N=71 among (Nos 66-429, 9001-9008). Table 3, col(1): <[FPH98] SMC NN> (Nos 1-27).
=E=	Catalogue in electronic form as J/A+AS/127/119
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPK2009]
[FPK2009]	(Fittingoff+Prochaska+Kalirai+, 2009)= (GALEX)
Write:	<<[FPK2009] GALEX JHHMMSS.ss+DDMMSS.s>> <<[FPK2009] JHHMMSS+DDMMSS>>
N:	98628+75+60
Object:	(UV) + QSO + AGN + G (SIMBAD class: UV = UV-emission Source)
Note:	GALEX and WIYN photometric and Lick 3m telescope spectroscopic observations of M31's extended halo.
in source:	M 31 = NGC 224
Ref:	=2009MNRAS.399..728F
by	FITTINGOFF A. , PROCHASKA J.X., KALIRAI J.S., STRADER J., GUHATHAKURTA P., KAPLAN K.F.
	Mon. Not. R. Astron. Soc., 399, 728-736 (2009)
	A survey of ultraviolet-bright sources behind the halo of M31.
o	Table 2: <[FPK2009] GALEX JHHMMSS.ss+DDMMSS.s> N=98628. Tables 4-5: <[FPK2009] JHHMMSS+DDMMSS> N=75+60.
=E=	Catalogue in electronic form as <J/MNRAS/399/728/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPK96]
[FPK96]	(Forbes+Phillips+Koo+, 1996)
Write:	<<[FPK96] NN>> <<[FPK96] JHHMMSS.s+DDMMSS>>
N:	18
Object:	G (SIMBAD class: Galaxy)
Note:	HST WFPC2 observations
Ref:	=1996ApJ...462...89F
by	FORBES D.A. , PHILLIPS A.C., KOO D.C., ILLINGWORTH G.D.
	Astrophys. J., 462, 89-103 (1996)
	Keck spectroscopy and Hubble Space Telescope imaging of field galaxies at moderate redshift.
o	Table 1: <[FPK96] NN> (Nos 1-18) = <[FPK96] JHHMMSS.s+DDMMSS>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPL2007]
[FPL2007]	(Fox+Petitjean+Ledoux+, 2007)= ([FPL2007a]) (Not yet in Simbad)
Write:	<<[FPL2007] QSO JHHMM+DDMMA abs N.NNN>>
N:	12
Object:	DLA
Note:	VLT UVES observations.
Ref:	=2007A&A...465..171F
by	FOX A.J. , PETITJEAN P., LEDOUX C., SRIANAND R.
	Astron. Astrophys., 465, 171-184 (2007)
	Hot halos around high redshift protogalaxies. Observations of OVI and NV absorption in damped Lyman-α systems.
o	Table 1: <[FPL2007] QSO JHHMM+DDMM abs N.NNN> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPL2007a]
[FPL2007a]	(Fox+Petitjean+Ledoux+, 2007) (Not yet in Simbad)
*****	Avoid the usage of [FPL2007a], prefer [FPL2007]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPL2007b]
[FPL2007b]	(Fox+Petitjean+Ledoux+, 2007) (Not yet in Simbad)
Write:	<<[FPL2007b] QSO J0332-4455 abs N.NNNNN>> <<[FPL2007b] QSO J0332-4455 abs N.NNN>>
N:	1+3
Object:	DLA + Sub-DLA
Note:	VLT UVES spectrum of QSO J0332-4455.
Ref:	=2007ApJ...668L..15F
by	FOX A.J. , PETITJEAN P., LEDOUX C., SRIANAND R.
	Astrophys. J., 668L, 15-18 (2007)
	Multiphase plasma in sub-damped Lyα systems: a hidden metal reservoir.
o	Table 1: <[FPL2007] QSO J0332-4455 abs N.NNNNN> N=1. Table 2: <[FPL2007] QSO J0332-4455 abs N.NNN> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FPM
FPM	(Frew+Parker+Miszalski)
Write:	<<FPM JHHMM+DDMM>>
N:	2
Object:	PN (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
Stat:	is completely incorporated in Simbad
Note:	Object name consists of the initial letters of the discoverers. See also BMP, MPA.
Ref:	=2008MNRAS.384..525M
by	MISZALSKI B. , PARKER Q.A., ACKER A., BIRKBY J.L., FREW D.J., KOVACEVIC A.
	Mon. Not. R. Astron. Soc., 384, 525-534 (2008)
	MASH-II: more planetary nebulae from the AAO/UKST Hα survey.
o	Table 3: <BMP JHHMM+DDMM> N=78, <FPM JHHMM+DDMM> N=2, <MPA JHHMM+DDMMa> N=255.
=E=	Catalogue in electronic form as V/127
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FPM
FPM	(Forbrich+Preibisch+Menten)
*****	Avoid the usage of FPM, prefer [FPM2006]
Origin	of the Acronym: L (2008ApJ...687..406C)
Details on Acronym: [FPM2006]
[FPM2006]	(Forbrich+Preibisch+Menten, 2006)= (FPM)
Write:	<<[FPM2006] NN>>
N:	15
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	VLA observations of the Coronet cluster, and analyse of archival Chandra and XMM-Newton data. See also [B87], [TS84], [FCW98].
in source:	Coronet Cluster = R CRa Cluster
Ref:	=2006A&A...446..155F
by	FORBRICH J. , PREIBISCH T., MENTEN K.M.
	Astron. Astrophys., 446, 155-170 (2006)
	Radio and X-ray variability of young stellar objects in the Coronet cluster.
o	Table 3: <[FPM2006] NN> (Nos 1-15). Table 3: <[TS84] IRS NNW> (Nos 7E, 7W) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPM88]
[FPM88]	(Fort+Prieur+Mathez+, 1988)
Write:	<<[FPM88] AN>>
N:	21
Object:	Arc + Blue obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	(Nos A1-A6) are 6 arcs in ACO 370. The giant arc in ACO 370 (cited in 1988A&A...191L..19S) is found later in the literature as No. 'A0'. (Nos B1-B4) are blue objects. (Nos C1-C4), (Nos D1-D3), (Nos E1-E3). Figs 1, 2: maps. See also [KMF94] and [SDK96].
in source:	ACO 370
Ref:	=1988A&A...200L..17F
by	FORT B. , PRIEUR J.L., MATHEZ G., MELLIER Y., SOUCAIL G.
	Astron. Astrophys., 200, 17-20 (1988)
	Faint distorted structures in the core of A 370: are they gravitationally lensed galaxies at z=1 ?
o	The giant arc in ACO 370 is found later in literature as [FPM88] A0
o	Tables I, and fig.1,2: <[FPM88] AN> (Nos A1-A6), (Nos B1-B3)
Ref:	=1993A&A...273..367K
by	KNEIB J.-P. , MELLIER Y., FORT B., MATHEZ G.
	Astron. Astrophys., 273, 367-None (1993)
	The distribution of dark matter in distant cluster-lenses: modelling A 370.
o	AC 114 = ACCG 114
o	Figs 1, 2: <[FPM88] AN> (No. B4), (Nos C1-C3), (Nos D1-D3).
Ref:	=1999A&A...347...21B
by	BEZECOURT J. , KNEIB J.P., SOUCAIL G., EBBELS T.M.D.
	Astron. Astrophys., 347, 21-29 (1999)
	Lensed galaxies in Abell 370. I. Modeling the number counts and redshift distribution of background sources.
o	Table 1, Fig.1: <[FPM88] AN> (Nos C4, E1-E3) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPQ2019]
[FPQ2019]	(Frye+Pascale+Qin+, 2019)
Write:	<<[FPQ2019] GLLL DSFG Na>> <<[FPQ2019] G165 NNa>> <<[FPQ2019] sNN>>
N:	12+28+62
Object:	Grav. lensed image of a G + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST WFC3-IR, LBT LUCI, Spitzer IRAC, MMT Hectospec, and Gemini-North GMOS observations of N=12 lensed images of dusty star-forming galaxies (DFSGs) in six fields, as well as N=28 additional lensed images and N=62 galaxies in the field of the lensed galaxie [CNG2015] PLCK G165.7+67.0.
Ref:	=2019ApJ...871...51F
by	FRYE B.L. , PASCALE M., QIN Y., ZITRIN A., DIEGO J., WALTH G., YAN H., CONSELICE C.J., ALPASLAN M., BAUER A., BUSONI L., COE D., COHEN S.H., DOLE H., DONAHUE M., GEORGIEV I., JANSEN R.A., LIMOUSIN M., LIVERMORE R., NORMAN D., RABIEN S., WINDHORST R.A.
	Astrophys. J., 871, 51-51 (2019)
	PLCK G165.7+67.0: analysis of a massive lensing cluster in a Hubble Space Telescope census of submillimeter giant arcs selected using Planck/Herschel.
o	Sources 2a and 2c have been reversed between Table 3 and Figures 8 and 9. The identification chosen in SIMBAD is that of the table.
o	Table 2: <[FPQ2019] GLLL DSFG Na> N=12. Fig. 8, Table 3: <[FPQ2019] G165 NNa> N=28 among (Nos 2a-2c to 11a-11c). Table 4: <[FPQ2019] sNN> (Nos s1-s62).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPR90]
[FPR90]	(Felli+Persi+Roth+, 1990)= (VLA)
Write:	<<[FPR90] G353.2+0.9 A>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
in source:	NGC 6357
in source:	GAL 353.2+00.9
Ref:	=1990A&A...232..477F
by	FELLI M. , PERSI P., ROTH M., TAPIA M., FERRARI-TONIOLO M., CERVELLI A.
	Astron. Astrophys., 232, 477-None (1990)
	Radio continuum, IR and CCD images of selected regions in NGC 6357.
o	Table 6: <[PFR86] G353.19+0.91 Irs N> (Nos 6-8) added. Table 7: <[FPR90] G353.2+0.9 A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPR99]
[FPR99]	(Fassnacht+Pearson+Readhead+, 1999)
Write:	<<[FPR99] 1608+656 W>> <<[FPR99] Source N>>
N:	2+4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Fig.2, Table 2: N=2 Northern and Southern radio lobes of the lens system CLASS B1608+656, already described in 1995ApJ...447L...9S. N=4 sources in the field of CLASS B1608+656. See also [MFD95], [KF99].
in source:	CLASS B1608+656
Ref:	=1999ApJ...527..498F
by	FASSNACHT C.D. , PEARSON T.J., READHEAD A.C.S., BROWNE I.W.A., KOOPMANS L.V.E., MYERS S.T., WILKINSON P.N.
	Astrophys. J., 527, 498-512 (1999)
	A determination of H_{0} with the CLASS gravitational lens B1608+656. I. Time delay measurements with the VLA.
o	p.499: calibrator 1633+741 not identified. Table 2: components 'A' = [MFD95] 1608+656 A.
o	Fig.2, Table 2: <[FPR99] 1608+656 W> (Nos N, S), <[FPR99] Source N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPS2000]
[FPS2000]	(Forbes+Polehampton+Stevens+, 2000) (Not yet in Simbad)
Write:	<<[FPS2000] Opt SS.ss-SS.s>> <<[FPS2000] IR SS.sss-SS.ss>> <<[FPS2000] Rad SS.sss-SS.ss>>
N:	17+14+16
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 2: Optical sources in the field of NGC 253. Table 3: IR/mm sources in the field of NGC 253. Table 4: Radio-sources in the field of NGC 253.
in source:	NGC 253
Ref:	=2000MNRAS.312..689F
by	FORBES D.A. , POLEHAMPTON E., STEVENS I.R., BRODIE J.P., WARD M.J.
	Mon. Not. R. Astron. Soc., 312, 689-697 (2000)
	A multiwavelength view at the heart of the superwind in NGC253.
o	Table 2: <[FPS2000] Opt SS.ss-SS.s> N=15. Table 3: <[FPS2000] IR SS.sss-SS.ss> N=17. Table 4: <[FPS2000] Rad SS.sss-SS.ss> N=16.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPS2003]
[FPS2003]	(Fox+Price+Soderberg+, 2003)= ([FPS2003a])
Write:	<<[FPS2003] SN>>
N:	2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	1.2 m Palomar telescope observations with NEAT camera. N=2 secondary standard stars in the field of GRB 021211.
Ref:	=2003ApJ...586L...5F
by	FOX D.W. , PRICE P.A., SODERBERG A.M., BERGER E., KULKARNI S.R., SARI R., FRAIL D.A., HARRISON F.A., YOST S.A., MATTHEWS K., PETERSON B.A., TANAKA I., CHRISTIANSEN J., MORIARTY-SCHIEVEN G.H.
	Astrophys. J., 586, 5-8 (2003)
	Discovery of early optical emission from GRB 021211.
o	p. L6 : Calibrator PKS 0734+100 not identified
o	Fig.1: <[FPS2003] SN> (Nos S1-S2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPS2003a]
[FPS2003a]	(Fox+Price+Soderberg+, 2003)
*****	Avoid the usage of [FPS2003a], prefer [FPS2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPS2003b]
[FPS2003b]	(Foley+Papenkova+Swift+, 2003)
Write:	<<[FPS2003b] NN>>
N:	11
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	KAIT Lick observations. N=11 stars in the field of SN 2002AP.
Ref:	=2003PASP..115.1220F
by	FOLEY R.J. , PAPENKOVA M.S., SWIFT B.J., FILIPPENKO A.V., LI W., MAZZALI P.A., CHORNOCK R., LEONARD D.C., VAN DYK S.D.
	Publ. Astron. Soc. Pac., 115, 1220-1235 (2003)
	Optical photometry and spectroscopy of the SN 1998bw-like type Ic supernova 2002ap.
o	Table 1, Fig.1: <[FPS2003b] NN> (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPS2006]
[FPS2006]	(Franciosini+Pallavicini+Sanz-Forcada, 2006)= ([FPS2006a]) = (NX)
Write:	<<[FPS2006] NX NNN>>
N:	174
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton observations of Sigma Orionis Cluster. X-ray sources with at least one cluster member or candidate within 5arcsec. See also [LC2008].
in source:	NAME sig Ori Cluster
Ref:	=2006A&A...446..501F
by	FRANCIOSINI E. , PALLAVICINI R., SANZ-FORCADA J.
	Astron. Astrophys., 446, 501-513 (2006)
	XMM-Newton observations of the σ Orionis cluster. II. Spatial and spectral analysis of the full EPIC field.
o	Tables A1, B: <[FPS2006] NX NNN> (Nos 1-174). Tables A1, A2: <[W96] NNNN-NNNN> N=24 added, <[W96] rJHHMMSS+DDMMa> N=7 added, <[W96] pJHHMMSS+DDMM> N=9 added.
=E=	Catalogue in electronic form as J/A+A/446/501
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPS2006a]
[FPS2006a]	(Franciosini+Pallavicini+Sanz-Forcada, 2006)
*****	Avoid the usage of [FPS2006a], prefer [FPS2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPS2006b]
[FPS2006b]	(Fesen+Pavlov+Sannwal, 2006)
Write:	<<[FPS2006b] JHHMMSS.ss+DDMMSS.s>> <<[FPS2006b] Star A>> <<[FPS2006b] Star N>>
N:	3+3+2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	HST NICMOS and STIS observtions.88 Stars around the SNE Cas A.
Ref:	=2006ApJ...636..848F
by	FESEN R.A. , PAVLOV G.G., SANWAL D.
	Astrophys. J., 636, 848-858 (2006)
	Near-infrared and optical limits for the central X-ray point source in the Cassiopeia A supernova remnant.
o	Table 3: "MDM NNNN" id not used in SIMBAD internal Michigan Darthmouth MIT id), but [ FPS2006b] with coordinates.
o	Table 3: <[FPS2006b] JHHMMSS.ss+DDMMSS.s> N=3. Table 4, Fig.2: <[FPS2006b] Star A> (Nos A-B), <[FPS2006b] Star N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPS2016]
[FPS2016]	(Flores-Cacho+Pierini+Soucail+, 2016)
Write:	<<[FPS2016] ANa>>
N:	13
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT X-Shooter spectroscopic observations of N=13 galaxies.
Ref:	=2016A&A...585A..54F
by	FLORES-CACHO I. , PIERINI D., SOUCAIL G., MONTIER L., DOLE H., POINTECOUTEAU E., PELLO R., LE FLOC'H E., NESVADBA N., LAGACHE G., GUERY D., CANAMERAS R.
	Astron. Astrophys., 585A, 54-54 (2016)
	Multi-wavelength characterisation of z ~ 2 clustered, dusty star-forming galaxies discovered by Planck.
o	Table 1: <[FPS2016] Ana> N=13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPT2004]
[FPT2004]	(Francis+Palunas+Teplitz+, 2004)
Write:	<<[FPT2004] JHHMMSS.ss+DDMMSS.s>>
N:	58+43
Object:	poss. QSO + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Spectroscopy with the 2dF multifiber spectrograph. N=58 QSOs and N=43 foreground galaxies in the region containing the ClG J2143-4423 (cluster at z=2.38). See also [FWW96], [PTF2004].
Ref:	=2004ApJ...614...75F
by	FRANCIS P.J. , PALUNAS P., TEPLITZ H.I., WILLIGER G.M., WOODGATE B.E.
	Astrophys. J., 614, 75-83 (2004)
	The distribution of lyα-emitting galaxies at z=2.38. II. Spectroscopy.
o	Table 1: No. B6 is not the same as in 2004ApJ...602..545P, so this new object is designated as [FWW96] B6' in SIMBAD. Table 2: [FWW96] B6 (from 2004ApJ...602..545P) = [FWW96] 22 here. Table 1, Fig.7: objects b184, u093, u143, u194, P13 not identified.
o	Tables 1, 2: <[FWW96] ANN> N=22 among (Nos B10-B40), <[FWW96] AN'> (No. B6'). Tables 3, 4: <[FPT2004] JHHMMSS.ss+DDMMSS.s> N=58+43.
=E=	Catalogue in electronic form as J/ApJ/614/75
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPT95]
[FPT95]	(Falomo+Pesce+Treves, 1995)
Write:	<<[FPT95] PKS 0548-322 GN>>
N:	7
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	SUSI NTT observations. N=7 companion galaxies around PKS 0548-322.
Ref:	=1995ApJ...438L...9F
by	FALOMO R. , PESCE J.E., TREVES A.
	Astrophys. J., 438, 9-12 (1995)
	Host galaxy and environment of the BL Lacertae object PKS 0548-322 : observations with subarcsecond resolution.
o	Fig.1, Table 1: <[FPT95] PKS 0548-322 GN> (Nos G1-G7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FPU2013]
[FPU2013]	(Forbes+Pota+Usher+, 2013) (Not yet in Simbad)
Write:	<<[FPU2013] acsNNN>>
N:	12
Object:	Cluster of * + G (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Use of HST ACS data to search for star clusters in NGC 4697.
in source:	NGC 4697
Ref:	=2013MNRAS.435L...6F
by	FORBES D.A. , POTA V., USHER C., STRADER J., ROMANOWSKY A.J., BRODIE J.P., ARNOLD J.A., SPITLER L.R.
	Mon. Not. R. Astron. Soc., 435L, 6-10 (2013)
	Filling the gap: a new class of old star cluster?
o	Table A1: <[FPU2013] acsNNN> N=12+2 among (Nos 52-868).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FQS
FQS	(Forgotten Quadrant Survey)
Write:	<<FQS -MCLLL.lll+BB.bbb>> <<FQS -MCLLL.lll+B.bbb>> (not recognised by Simbad, but found in literature)
N:	263
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	The Forgotten Quadrant Survey (FQS) is an ESO large project that used the 12m antenna of the Arizona Radio Observatory to map the Galactic plane in the range 220°<l<240° and -2.5°<b<0°, both in 12CO(1-0) and 13CO(1-0), at a spectral resolution of 0.65km/s and 0.26km/s. A catalogue of N=263 molecular clouds is published as part of the first data release.
Ref:	=2020A&A...633A.147B
by	BENEDETTINI M. , MOLINARI S., BALDESCHI A., BELTRAN M.T., BRAND J., CESARONI R., ELIA D., FONTANI F., MERELLO M., OLMI L., PEZZUTO S., RYGL K.L.J., SCHISANO E., TESTI L., TRAFICANTE A.
	Astron. Astrophys., 633A, 147-147 (2020)
	The Forgotten Quadrant Survey. ^{12}CO and ^{13}CO (1-0) survey of the Galactic plane in the range 220° <l < 240° -2.5° < b < 0°.
o	Table A.1: <FQS-MCLLL.lll+BB.bbb> N=263.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FR
FR	(Folamont+Rogstad)
Write:	<<FR NNN>>
N:	120
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Ref:	=1966ApJ...146..528F
by	FOMALONT E.B. , ROGSTAD D.H.
	Astrophys. J., 146, 528-541 (1966)
	Radio emission from clusters of galaxies.
o	Table 1: <FR NNN> (Nos 1-120)
Origin	of the Acronym: L (1978A&AS...31...99H)
Details on Acronym: [FR2007]
[FR2007]	(Fish+Reid, 2007) (Not yet in Simbad)
Write:	<<[FR2007] NNN>>
N:	123
Object:	OH Maser Spot (SIMBAD class: Maser)
Note:	VLBA observations of the 1665 and 1667MHz OH masers in the massive star-forming region W 75N.
in source:	W 75:W 75N = W 75N
Ref:	=2007ApJ...656..952F
by	FISH V.L. , REID M.J.
	Astrophys. J., 656, 952-958 (2007)
	Large magnetic fields and motions of OH masers in W75N.
o	Table 1: <[FR2007] NNN> (Nos 1-123).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FR78]
[FR78]	(Feast+Robertson, 1978) (Not yet in Simbad)
Write:	<<[FR78] A>>
N:	6
Object:	Feature (SIMBAD class: PartofG = Part of a Galaxy)
in source:	NGC 3256
Ref:	=1978MNRAS.185...31F
by	FEAST M.W. , ROBERTSON B.S.C.
	Mon. Not. R. Astron. Soc., 185, 31-46 (1978)
	The kinematics of the peculiar galaxy NGC 3256.
o	Plate 1: <[FR78] A> (Nos S, T, W-Z).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FRA2004]
[FRA2004]	(Frayer+Reddy+Armus+, 2004)
Write:	<<[FRA2004] AN>> <<[FRA2004] BN>>
N:	3+1
Object:	(Near IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Used of the NIR Camera on the Keck I telescope to search for new possible counterpart of SMM galaxies from the SCUBA Lens Survey. Format 'AN' with the letter 'A' for new possible counterparts, A1 and A2 for [SIB98] SMM J02400-0134, A3 for [SIB98] SMM J22472-0206. Format 'B1' for additional source with extremely red NIR color in the field of an SMM galaxy: B1 is 4" northeast of [BCS99b] Cl 0939+47 H5. See also [BCS99b]
Ref:	=2004AJ....127..728F
by	FRAYER D.T. , REDDY N.A., ARMUS L., BLAIN A.W., SCOVILLE N.Z., SMAIL I.
	Astron. J., 127, 728-735 (2004)
	Near-infrared colors of submillimeter-selected galaxies.
o	Table 2: <[FRA2004] AN> (Nos A1-A3, B1). Table 2: <[BCS99b] ACO 1835 J1a> (No. J1a) added, <[BCS99b] Cl 2244-02 ANa> (Nos P1a, P1b, P7) added, <[BCS99b] ACO 2390 ANa> (Nos K3a, K3b) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FRB
FRB	(Fast Radio Burst)
Write:	<<FRB YYMMDD>> <<FRB YYYYMMDDA>> <<FRB YYYYMMDDaaa>>
Object:	(Radio) (SIMBAD class: Radio = Radio Source)
Note:	A fast radio burst (FRB) is a transient radio pulse lasting only a few milliseconds. Since about 2020, FRB names are provided by the Transient Name Server (TNS, https://www.wis-tns.org), the official IAU mechanism for reporting new astronomical transients.
Details on Acronym: [FRB2004]
[FRB2004]	(Ferdman+Richer+Brewer+, 2004)
Write:	<<[FRB2004] PC NNN>> <<[FRB2004] WFN NNN>>
N:	47
Object:	* in Cl* (SIMBAD class: Star)
Note:	HST observations of M 4 to search for variable objects.
Ref:	=2004AJ....127..380F
by	FERDMAN R.D. , RICHER H.B., BREWER J., FAHLMAN G.G., GIBSON B.K., HANSEN B.M.S., HUBER M.E., IBATA R.A., KALIRAI J.S., MATTHEWS J.M., RICH R.M., ROWE J.F., SHARA M.M., STETSON P.B.
	Astron. J., 127, 380-393 (2004)
	Searching for variability in the globular cluster Messier 4.
o	Tables 2, 3, 4: <[FRB2004] PC NNN>, <[FRB2004] WF2 NNN>, <[FRB2004] WF3 NNN>, <[FRB2004] WF4 NNN>, N=47.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FRB2008]
[FRB2008]	(Freire+Ransom+Begin+, 2008)
Write:	<<[FRB2008] JHHMM+DDMMA>> <<[FRB2008] NGC NNNNA>>
N:	6+4
Object:	ms Psr (SIMBAD class: Pulsar)
Stat:	is completely incorporated in Simbad
Note:	GBT systematic search for millisecond pulsars in NGC 6440 and NGC 6441.
in source:	NGC 6440
in source:	NGC 6441
Ref:	=2008ApJ...675..670F
by	FREIRE P.C.C. , RANSOM S.M., BEGIN S., STAIRS I.H., HESSELS J.W.T., FREY L.H., CAMILO F.
	Astrophys. J., 675, 670-682 (2008)
	Eight new millisecond pulsars in NGC 6440 and NGC 6441.
o	Tables 3, 4: <[FRB2008] J1748-2021A> (Nos A-F) = <[FRB2008] NGC 6440A> (Nos A-F), <[FRB2008] J1750-3703A> (Nos A-D) = <[FRB2008] NGC 6441A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FRD2013]
[FRD2013]	(Fallscheer+Reid+Di Francesco+, 2013)
Write:	<<[FRD2013] HMDC NN>> <<[FRD2013] HMDC A>>
N:	13+3
Object:	Clump (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	Herschel HOBYS observations of N=13 high-mass dense clump candidate in the nearby high-mass star-forming region NGC 7538.
in source:	[FRD2013]
Ref:	=2013ApJ...773..102F
by	FALLSCHEER C. , REID M.A., DI FRANCESCO J., MARTIN P.G., HILL T., HENNEMANN M., NGUYEN-LUONG Q., MOTTE F., MEN'SHCHIKOV A., ANDRE Ph., WARD-THOMPSON D., GRIFFIN M., KIRK J., KONYVES V., RYGL K.L.J., SADAVOY S., SAUVAGE M., SCHNEIDER N., ANDERSON L.D., BENEDETTINI M., BERNARD J.-P., BONTEMPS S., GINSBURG A., MOLINARI S., POLYCHRONI D., RIVERA-INGRAHAM A., ROUSSEL H., TESTI L., WHITE G., WILLIAMS J.P., WILSON C.D., WONG M., ZAVAGNO A.
	Astrophys. J., 773, 102 (2013)
	Herschel reveals massive cold clumps in NGC 7538.
o	Table 1: <[FRD2013] HMDC NN> (Nos 1-13), Fig. 5: <[FRD2013] HMDC A> N=3 (Nos A, B, C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FRG92]
[FRG92]	(Friedemann+Reimann+Gurtler, 1992)
Write:	<<[FRG92] a>>
N:	13
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=13 comparison stars used for SV Cephei, (Nos a-m). Identif. chart in Fig.1. They are coming from an atlas of Papadopoulos+, 1980. Updated version in 1999A&AS..140..293G: [GFR99]. Coordinates and missing letters added in 2000ARep...44..365R.
Ref:	=1992A&A...255..246F
by	FRIEDEMANN C. , REIMANN H.-G., GURTLER J.
	Astron. Astrophys., 255, 246-254 (1992)
	A cloudy circumstellar dust shell around SV Cephei.
o	Table 2: <[FRG92] a> N=10 among (Nos b-m>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FRH2008]
[FRH2008]	(Fesen+Rudie+Hurford+, 2008) (Not yet in Simbad)
Write:	<<[FRH2008] NAaa>>
N:	463
Object:	Em. Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Spectroscopic survey of optical emission knots associated with the SNR 3C 58.
in source:	3C 58
Ref:	=2008ApJS..174..379F
by	FESEN R. , RUDIE G., HURFORD A., SOTO A.
	Astrophys. J., Suppl. Ser., 174, 379-395 (2008)
	Optical imaging and spectroscopy of the galactic supernova remnant 3C 58 (G130.7+3.1).
o	Table 2: <[FRH2008] NAaa> N=463.
=E=	Catalogue in electronic form as J/ApJS/174/379
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FRK2004]
[FRK2004]	(Foster+Routledge+Kothes, 2004)
Write:	<<[FRK2004] NN>>
N:	11
Object:	* (SIMBAD class: Star)
Note:	Optical observations at the 0.5m telescope at the University of Alberta's Devon Astronomical Observatory. N=11 stars in the field of 3C 434.1.
Ref:	=2004A&A...417...79F
by	FOSTER T. , ROUTLEDGE D., KOTHES R.
	Astron. Astrophys., 417, 79-91 (2004)
	The Galactic Plane region near l=93°. II. A stellar wind bubble surrounding SNR 3C434.1.
o	Tables 3, 4: <[FRK2004] NN> (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Frl
Frl	(Fairall)= (F) = (Fa) = (Fair) = (Fairall)
Write:	<<Frl NNNN>>
N:	1185
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Ref:	=1977MNRAS.180..391F
by	FAIRALL A.P.
	Mon. Not. R. Astron. Soc., 180, 391-400 (1977)
	150 southern compact and bright-nucleus galaxies.
o	Table 1: <Frl NNN> (Nos 1-150)
Ref:	=1979MNRAS.188..349F
by	FAIRALL A.P.
	Mon. Not. R. Astron. Soc., 188, 349-356 (1979)
	Spectroscopic survey of southern compact and bright-nucleus galaxies. II.
o	Table 2: <Frl NNN> (Nos 151-210)
Ref:	=1980MNRAS.192..389F
by	FAIRALL A.P.
	Mon. Not. R. Astron. Soc., 192, 389-397 (1980)
	Spectroscopic survey of southern compact and bright-nucleus galaxies. III.
o	Table 2: <Frl NNN> (Nos 211-290)
Ref:	=1981MNRAS.196..417F
by	FAIRALL A.P.
	Mon. Not. R. Astron. Soc., 196, 417-424 (1981)
	Spectroscopic survey of southern compact and bright-nucleus galaxies. IV.
o	Table 1: <Frl NNN> (Nos 291-360)
Ref:	=1983MNRAS.203...47F
by	FAIRALL A.P.
	Mon. Not. R. Astron. Soc., 203, 47-54 (1983)
	Spectroscopic survey of southern compact and bright-nucleus galaxies. V.
o	Table 1: <Frl NNN> (Nos 361-625)
Ref:	=1984MNRAS.210...69F
by	FAIRALL A.P.
	Mon. Not. R. Astron. Soc., 210, 69-77 (1984)
	Spectroscopic survey of southern compact and bright-nucleus galaxies - VI.
o	Table 1: <Frl NNNN> (Nos 626-1065)
Ref:	=1988MNRAS.233..691F
by	FAIRALL A.P.
	Mon. Not. R. Astron. Soc., 233, 691-696 (1988)
	Spectroscopic survey of southern compact and bright nucleus galaxies - VII.
o	Table 1: <Frl NNNN> (Nos 1066-1185)
Details on Acronym: [FRM2008]
[FRM2008]	(Finkelstein+Rhoads+Malhotra+, 2008)
Write:	<<[FRM2008] Object N>>
N:	6
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	CTIO 4m Blanco telescope Halpha observations to search for Lyman-alpha galaxies in the CDFS. Use of archival GOODS HST and Chandra data.
in source:	NAME CDFS
Ref:	=2008ApJ...678..655F
by	FINKELSTEIN S.L. , RHOADS J.E., MALHOTRA S., GROGIN N., WANG J.
	Astrophys. J., 678, 655-668 (2008)
	Effects of dust geometry in Lyα galaxies at z = 4.4.
o	Table 1: <[FRM2008] Object N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FRM2009]
[FRM2009]	(Finkelstein+Rhoads+Malhotra+, 2009)= (CHa)
Write:	<<[FRM2009] CHa-N>> <<[FRM2009] CH8-N>> <<[FRM2009] CS2-N>>
N:	4+2+8
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	CTIO 4m Blanco telescope Halpha observations to search for Lyman-alpha galaxies in the CDFS. Use of archival HST and Spitzer data.
in source:	NAME CDFS
Ref:	=2009ApJ...691..465F
by	FINKELSTEIN S.L. , RHOADS J.E., MALHOTRA S., GROGIN N.
	Astrophys. J., 691, 465-481 (2009)
	Lyman α galaxies: primitive, dusty, or evolved?
o	Table 1: <[FRM2009] CHa-N> (Nos 1-4), <[FRM2009] CH8-N> (Nos 1-2), <[FRM2009] CS2-N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FRM2016]
[FRM2016]	(Forbrich+Rivilla+Menten+, 2016)
Write:	<<[FRM2016] NNN>>
N:	556
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 4.7 and 7.3GHz continuum observations of N=556 compact sources in the Orion Nebula Cluster.
in source:	NAME Orion Nebula Cluster
Ref:	=2016ApJ...822...93F
by	FORBRICH J. , RIVILLA V.M., MENTEN K.M., REID M.J., CHANDLER C.J., RAU U., BHATNAGAR S., WOLK S.J., MEINGAST S.
	Astrophys. J., 822, 93-93 (2016)
	The population of compact radio sources in the Orion Nebula Cluster.
o	Table 1: <[FRM2016] NNN> (Nos 1-556).
=E=	Catalogue in electronic form as <J/ApJ/822/93/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FRM2018]
[FRM2018]	(Forster Schreiber+Renzini+Mancini+, 2018) (Not yet in Simbad)
Write:	<<[FRM2018] ZC400569N>> <<[FRM2018] {ZC407376N\|ZC407376S}>>
N:	1+2
Object:	G (SIMBAD class: Galaxy)
Note:	VLT SINFONI observations of N=3 galaxies from the SINS/zC-SINF AO survey. See also [MFR2011b].
in source:	COSMOS2015 300906
in source:	UVISTADR1 J100045.14+020705.2
Ref:	=2018ApJS..238...21F
by	FORSTER SCHREIBER N.M. , RENZINI A., MANCINI C., GENZEL R., BOUCHE N., CRESCI G., HICKS E.K.S., LILLY S.J., PENG Y., BURKERT A., CAROLLO C.M., CIMATTI A., DADDI E., DAVIES R.I., GENEL S., KURK J.D., LANG P., LUTZ D., MAINIERI V., McCRACKEN H.J., MIGNOLI M., NAAB T., OESCH P., POZZETTI L., SCODEGGIO M., SHAPIRO GRIFFIN K., SHAPLEY A.E., STERNBERG A., TACCHELLA S., TACCONI L.J., WUYTS S., ZAMORANI G.
	Astrophys. J., Suppl. Ser., 238, 21-21 (2018)
	The SINS/zC-SINF survey of z ~ 2 galaxy kinematics: SINFONI adaptive optics-assisted data and kiloparsec-scale emission-line properties.
o	Table 1: <[FRM2018] ZC400569N> N=1, <[FRM2018] ZC407376N> N=1, <[FRM2018] ZC407376S> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FRM2019]
[FRM2019]	(Fischer+Rigby+Mahler+, 2019)
Write:	<<[FRM2019] SGAS J0033+02 N.N>> <<[FRM2019] SGAS J0033+02 1a.N>>
N:	24+4
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Stat:	is completely incorporated in Simbad
Note:	HST WFC3, Magellan Baade telescope MagE, VLT SINFONI, and VLT MUSE observations of N=24+4 gravitationally lensed images of SGAS J003341.5+024217.
Ref:	=2019ApJ...875..102F
by	FISCHER T.C. , RIGBY J.R., MAHLER G., GLADDERS M., SHARON K., FLORIAN M., KRAEMER S., BAYLISS M., DAHLE H., BARRIENTOS L.F., LOPEZ S., TEJOS N., JOHNSON T., WUYTS E.
	Astrophys. J., 875, 102-102 (2019)
	Spatially resolved outflows in a Seyfert galaxy at z = 2.39.
o	Fig. 9, Table 2: <[FRM2019] SGAS J0033+02 N.N> N=24 among (Nos 1.1-1.4 to 9.1-9.3, <[FRM2019] SGAS J0033+02 1a.N> (Nos 1a.1-1a.4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FRM96]
[FRM96]	(Fuente+Rodriguez-Franco+Martin-Pintado, 1996)
Write:	<<[FRM96] AAN>>
N:	6+3
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Fig.2: N=6 Southern molecular Bars ('SB' in the format), (Nos SB1-SB6) and N=3 Northern molecular Bars ('NB' in the format), (Nos NB1-NB3)
in source:	NAME Orion Nebula
Ref:	=1996A&A...312..599F
by	FUENTE A. , RODRIGUEZ-FRANCO A., MARTIN-PINTADO J.
	Astron. Astrophys., 312, 599-609 (1996)
	Chemistry in the high density molecular interface surrounding the Orion nebula.
o	Fig.2: <[FRM96] SBN> (Nos SB1-SB6), <[FRM96] NBN> (Nos NB1-NB3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FRO
FRO	(Fleurs Radio Obs.) (Not yet in Simbad)
*****	Avoid the usage of FRO, prefer [FJ73]
Details on Acronym: [FRO2001]
[FRO2001]	(Farrah+Rowan-Robinson+Oliver+, 2001)
Write:	<<[FRO2001] IRAS HHMMm+DDMM A>>
N:	2x2
Object:	G in Pair (SIMBAD class: GinPair = Galaxy in Pair of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 images of IRAS ULIRGS with two clearly separated galaxies. 2 are binary systems.
in source:	IRAS 02587-6336
in source:	IRAS 20176-4756
Ref:	=2001MNRAS.326.1333F
by	FARRAH D. , ROWAN-ROBINSON M., OLIVER S., SERJEANT S., BORNE K., LAWRENCE A., LUCAS R.A., BUSHOUSE H., COLINA L.
	Mon. Not. R. Astron. Soc., 326, 1333-1352 (2001)
	HST/WFPC2 imaging of the QDOT ultraluminous infrared galaxy sample.
o	Table 2: IRAS 02587-4336 misprint for IRAS 02587-6336.
o	Table 2: <[FRO2001] IRAS 02587-6336 A> (Nos A-B), <[FRO2001] IRAS 20176-4756 A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Frolov
Frolov	(Frolov)
N:	1
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Stat:	is completely incorporated in Simbad
Ref:	=1977IzPul.195...80F
by	FROLOV V.N.
	Izv. Glav. Astron. Obs., 195, 80-97 (1977)
	Photometry and proper motions of stars of four galactic clusters in Cassiopeia.
o	Table 4: <Cl* NGC 7788 F NN> (Nos 1-67). Table 6: <Cl* NGC 7790 F NN> (Nos 1-60). Table 10: <Cl* Berkeley 58 F NN> (Nos 1-46). Table 11: <[F77] Frolov 1 NN> (Nos 1-27).
Details on Acronym: [FRP2000]
[FRP2000]	(Franciosini+Randich+Pallavicini, 2000)
Write:	<<[FRP2000] NN>>
N:	49
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations of NGC 3532. Among the 49 X-ray sources, 13 are probably not cluster members and 21 are unidentified.
in source:	NGC 3532
Ref:	=2000A&A...357..139F
by	FRANCIOSINI E. , RANDICH S., PALLAVICINI R.
	Astron. Astrophys., 357, 139-144 (2000)
	A ROSAT HRI study of the open cluster NGC 3532.
o	Tables 1-3: <[FRP2000] NN> (Nos 1-49).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FRP2003]
[FRP2003]	(Franciosini+Randich+Pallavicini, 2003)
Write:	<<[FRP2003] JHHMMSS.ss+DDMMSS.s>>
N:	24
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of the Hyades cluster. N=24 X-ray sources with at least an optical counterpart which is a cluster non-member or has no membership information.
Ref:	=2003A&A...405..551F
by	FRANCIOSINI E. , RANDICH S., PALLAVICINI R.
	Astron. Astrophys., 405, 551-561 (2003)
	Is Praesepe really different from the coeval Hyades cluster? The XMM-Newton view.
o	In table 3, GSC2 N231230081115 is a misprint for N23123008115. KW = Cl* NGC 2632 KW, JS = Cl* NGC 2632 JS, HSHJ = Cl* NGC 2632 HSHJ, WRS = Cl* NGC 2632 WRS in SIMBAD
o	Table 3: <[FRP2003] JHHMMSS.ss+DDMMSS.s> N=24.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FRP2015]
[FRP2015]	(Finkelstein+Ryan+Papovic+, 2015)
Write:	<<[FRP2015] zN AAA NNNNN>> <<[FRP2015] zN AAAA NNNNN>> <<[FRP2015] zN MACS0416PAR NNNNN>> <<[FRP2015] zN A2744PAR NNNNN>> <<[FRP2015] zN PARN NNNN>>
N:	7446
Object:	G (SIMBAD class: Galaxy)
Note:	N=7446 candidate galaxies at 3.5<z<8.5 in the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey/GOODS fields, the Hubble Ultra Deep Field, and the Hubble Frontier Field (HFF) deep parallel observations near the Abell 2744 and MACS J0416.1-2403 clusters. In the format, zN indicates the redshift range (z4 to z8), and AAA, AAA, MACS0416PAR or A2744PAR stand for the considered field (GSD -> GOODS-S Deep, GSW -> GOODS-S Wide, ERS -> GOODS-S ERS, GND -> GOODS-N Deep, GNW -> GOODS-N Wide, PAR1 and PAR2 -> HUDF parallel fields, Main -> HUDF Main, HUDF PAR1 and HUDF PAR2 -> HUDF Main field, MACS0416PAR and A2744PAR -> HFF parallel fields). Use of HST data from CANDELS, HUDF and HUDF09 surveys, and Frontier Fields program. See also <HRG14>.
in source:	NAME GOODS South Field
in source:	NAME GOODS North Field
in source:	NAME HUDF
in source:	MCS J0416.1-2403
in source:	ACO 2744
Ref:	=2015ApJ...810...71F
by	FINKELSTEIN S.L. , RYAN R.E.Jr, PAPOVICH C., DICKINSON M., SONG M., SOMERVILLE R.S., FERGUSON H.C., SALMON B., GIAVALISCO M., KOEKEMOER A.M., ASHBY M.L.N., BEHROOZI P., CASTELLANO M., DUNLOP J.S., FABER S.M., FAZIO G.G., FONTANA A., GROGIN N.A., HATHI N., JAACKS J., KOCEVSKI D.D., LIVERMORE R., McLURE R.J., MERLIN E., MOBASHER B., NEWMAN J.A., RAFELSKI M., TILVI V., WILLNER S.P.
	Astrophys. J., 810, 71 (2015)
	The evolution of the galaxy rest-frame ultraviolet luminosity function over the first two billion years.
o	Table 3, col(2): <HRG14 JHHMMSS.ss+DDMMSS.s> N=7446 = Table 3, col(1): <[FRP2015] zN AAAAAAAAAAA NNNNN>, <[FRP2015] zN PARN NNNN>, N=7446.
=E=	Catalogue in electronic form as J/ApJ/810/71
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FRS
FRS	(Faint Images of the Radio Sky at Twenty-cm)
*****	Avoid the usage of FRS, prefer FIRST
Origin	of the Acronym: L (2000ApJ...532..700A)
Details on Acronym: [FRS2006]
[FRS2006]	(Fliri+Riffeser+Seitz+, 2006)= ([FRS2006a]) = (WeCAPP)
Write:	<<[FRS2006] WeCAPP VNNNNN>>
N:	23781
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Wendelstein Calar Alto Pixellensing Project: catalogue of variable stars in the bulge of M 31.
in source:	M 31 = NGC 224
Ref:	=2006A&A...445..423F
by	FLIRI J. , RIFFESER A., SEITZ S., BENDER R.
	Astron. Astrophys., 445, 423-439 (2006)
	The Wendelstein Calar Alto Pixellensing Project (WeCAPP): the M 31 variable star catalogue.
o	Tables 2a (Cepheids) and 2b (Type II Cepheids) are ingested in SIMBAD.
o	Table 2: <[FRS2006] WeCAPP VNNNNN> (Nos V1-V23781).
=E=	Catalogue in electronic form as J/A+A/445/423
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FRS2006a]
[FRS2006a]	(Fliri+Riffeser+Seitz+, 2006)
*****	Avoid the usage of [FRS2006a], prefer [FRS2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FRS2006b]
[FRS2006b]	(Fechner+Reimers+Songaila+, 2006) (Not yet in Simbad)
Write:	<<[FRS2006b] QSO J1701+6412 abs N.NNNN>>
N:	25
Object:	Absorber
Note:	FUSE observations of the spectrum of HS 1700+6416 = QSO J1701+6412.
Ref:	=2006A&A...455...73F
by	FECHNER C. , REIMERS D., SONGAILA A., SIMCOE R.A., RAUCH M., SARGENT W.L.W.
	Astron. Astrophys., 455, 73-90 (2006)
	The UV spectrum of HS 1700+6416. I. Predicting the metal line content of the far UV spectrum.
o	Table 1: <[FRS2006b] QSO J1701+6412 abs N.NNNN> N=22.
Ref:	=2006A&A...455...91F
by	FECHNER C. , REIMERS D., KRISS G.A., BAADE R., BLAIR W.P., GIROUX M.L., GREEN R.F., MOOS H.W., MORTON D.C., SCOTT J.E., SHULL J.M., SIMCOE R., SONGAILA A., ZHENG W.
	Astron. Astrophys., 455, 91-106 (2006)
	The UV spectrum of HS 1700+6416. II. FUSE observations of the HeII Lyman α forest.
o	Text: <[FRS2006b] QSO J1701+6412 abs N.NNNN> N=3 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FRS79]
[FRS79]	(Fischer+Righini-Cohen+Simon, 1979)
Write:	<<[FRS79] N>>
N:	9
Object:	(Near IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Ref:	=1979AJ.....84.1574F
by	FISCHER J. , RIGHINI-COHEN G., SIMON M., CASSAR L.
	Astron. J., 84, 1574-1580 (1979)
	Far infrared, near infrared and radio molecular line studies of HFE 2, HFE 3 and FJM 6.
o	Table II: <[FRS79] N> (Nos 1-9)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FrSh
FrSh	(Frieswijk and Shipman High-resolution)
Write:	<<FrSh HNNNN>> <<FrSh LNNNN>>
N:	1320+1589
Object:	Cloud + Part of Cloud (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	We use the Mann-Whitney U-test, in combination with a friends-of-friends algorithm, to identify extended reddened regions in the outer galactic plane using the 2MASS all-sky J-H-K survey. We process the data at two different resolutions, resulting in a high- and low-resolution catalog (1320 objects at 60" and 1589 objects at 90", respectively). The majority of extended red regions are associated with major molecular cloud complexes, supporting the hypothesis that the reddening is mostly due to foreground clouds and embedded objects. (link to accepted, but not final paper: http://www.astro.rug.nl/~frieswyk/Data/Research/OGIRDC/PDF/mwu.pdf)
Ref:	=2010A&A...515A..51F
by	FRIESWIJK W.W.F. , SHIPMAN R.F.
	Astron. Astrophys., 515A, 51-51 (2010)
	Searching for dark clouds in the outer galactic plane. I. A statistical approach for identifying extended red(dened) regions in 2MASS.
o	Table 1: <FrSh HNNNN> (Nos H1-H1320), <FrSh LNNNN> (Nos L1-L1589).
=E=	Catalogue in electronic form as J/A+A/515/A51
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: FS
FS	(Feitzinger+Stuve)
*****	Avoid the usage of FS, prefer FeSt
Details on Acronym: FS
FS	(Faint Standard)
Write:	<<FS NNN>>
N:	33+55
Object:	Faint * (SIMBAD class: Star)
Note:	Faint Standard stars. From Casali+, unpublished: (Nos 1-35), Nos 8, 22 missing. (Nos 101-155) are added later in 2001MNRAS.325..563H.
Auth.:	CASALI M.+
Ref:	=2001MNRAS.325..563H
by	HAWARDEN T.G. , LEGGETT S.K., LETAWSKY M.B., BALLANTYNE D.R., CASALI M.M.
	Mon. Not. R. Astron. Soc., 325, 563-574 (2001)
	JHK standard stars for large telescopes: the UKIRT Fundamental and Extended lists.
o	in ref list Drilling, Landolt 1979AJ.....84..783D instead of ApJ.84.783
o	Table 1: <FS NNN> (Nos 101-155) added.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FS
FS	(Ferguson+Sandage)
*****	Avoid the usage of FS, prefer [FS90]
Origin	of the Acronym: L (1996ApJS..105..269H)
Details on Acronym: [FS2003]
[FS2003]	(Fuhrmeister+Schmitt, 2003)= ([FS2003a])
Write:	<<[FS2003] NNNN>>
N:	1207
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Systematic search for variability among ROSAT All-Sky Survey X-ray sources.
Ref:	=2003A&A...403..247F
by	FUHRMEISTER B. , SCHMITT J.H.M.M.
	Astron. Astrophys., 403, 247-260 (2003)
	A systematic study of X-ray variability in the ROSAT all-sky survey.
o	Table 7: <[FS2003] NNNN> (Nos 1-1207).
=E=	Catalogue in electronic form as J/A+A/403/247
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FS2003a]
[FS2003a]	(Fuhrmeister+Schmitt, 2003)
*****	Avoid the usage of [FS2003a], prefer [FS2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FS2003b]
[FS2003b]	(Froebrich+Scholz, 2003)
Write:	<<[FS2003b] NIR NN>> <<[FS2003b] H2-knot N>> <<[FS2003b] H2-knot N-a>> <<[FS2003b] Outflow N>>
N:	31+31+3
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Calar Alto observations Observations of IC 1396W globule: N=31 NIR young stars, N=31 new discovered H2 knots, and N=3 H2 outflows.
in source:	IC 1396W
Ref:	=2003A&A...407..207F
by	FROEBRICH D. , SCHOLZ A.
	Astron. Astrophys., 407, 207-212 (2003)
	Young stars and outflows in the globule IC 1396W.
o	Table 1: <[FS2003b] NIR NN> (Nos 1-31). Table 2: <[FS2003b] H2-knot N-a> (Nos 1-a to 1-h, 2-a to 2-n, 3-a to 3-f, 4 to 6). Fig.2: <[FS2003b] Outflow N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FS2007]
[FS2007]	(Fu+Stockton, 2007)= ([FS2007a]) (Not yet in Simbad)
Write:	<<[FS2007] 4C 37.43 a>>
N:	8
Object:	Cloud (SIMBAD class: Cloud)
Note:	Gemini and Keck II spectroscopy of the Extended Emission-Line Region (EELR) around 4C 37.43. See also [SMH2002].
in source:	NAME 4C 37.43 EELR
Ref:	=2007ApJ...666..794F
by	FU H. , STOCKTON A.
	Astrophys. J., 666, 794-805 (2007)
	Integral field spectroscopy of the extended emission-line region of 4C 37.43.
o	Table 1: <[SMH2002] 4C 37.43 W1> (Nos S1, N1) added. Table 1: <[FS2007] 4C 37.43 a> (Nos a-h).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FS2007a]
[FS2007a]	(Fu+Stockton, 2007) (Not yet in Simbad)
*****	Avoid the usage of [FS2007a], prefer [FS2007]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FS2007b]
[FS2007b]	(Fish+Sjouwerman, 2007) (Not yet in Simbad)
Write:	<<[FS2007b] NNN>>
N:	292
Object:	OH Maser Spot (SIMBAD class: Maser)
Note:	European VLBI Network.
in source:	W 3:W 3(OH) = W 3(OH)
Ref:	=2007ApJ...668..331F
by	FISH V.L. , SJOUWERMAN L.O.
	Astrophys. J., 668, 331-347 (2007)
	Structure of W3(OH) from very high spectral resolution observations of 5 centimeter OH masers.
o	Table 1: <[FS2007b] NNN> (Nos 1-292).
=E=	Catalogue in electronic form as J/ApJ/668/331
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FS2008]
[FS2008]	(Fu+Stockton, 2008)
Write:	<<[FS2008] 3C 79A>> <<[FS2008] a>> <<[FS2008] WN>>
N:	1+4+2
Object:	G + Cloud (SIMBAD class: Cloud)
Note:	Gemini GMOS, Keck I LRIS, and HST WFPC2 observations of the radio galaxy 3C 79: N=1 companion galaxy, and N=6 emission-line clouds are observed.
in source:	3C 79
Ref:	=2008ApJ...677...79F
by	FU H. , STOCKTON A.
	Astrophys. J., 677, 79-91 (2008)
	The host galaxy and the extended emission-line region of the radio galaxy 3C 79.
o	Table 1: <[FS2008] 3C 79A> N=1. Tables 2, 3: <[FS2008] a> (Nos a-d), <[FS2008] WN> (Nos N1, S1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FS83]
[FS83]	(Fried+Schulz, 1983)
Write:	<<[FS83] A R>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	NGC 6240 is a double nucleus galaxy, Nucleus I (N I) and Nucleus I (N II), also found in the literature as NGC 6240S and NGC 6240N.
in source:	NGC 6240
Ref:	=1983A&A...118..166F
by	FRIED J.W. , SCHULZ H.
	Astron. Astrophys., 118, 166-170 (1983)
	NGC 6240: a unique interacting galaxy.
o	<[FS83] A R> (Nos N I, N II).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FS90]
[FS90]	(Ferguson+Sandage, 1990)= (FS) = (LGC)
Write:	<<[FS90] Leo NN>> <<[FS90] Dorado NN>> <<[FS90] NGC 1400 NNN>> <<[FS90] NGC 5044 NNNA>> <<[FS90] Antlia NNN>>
N:	788+9
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Galaxies in 5 nearby groups. In NGC 5044 group, new dwarf galaxies are added in other refs, with the format 'NNNA', where 'NNN' is the nearest galaxy in the first ref. Also designated as FSG in SIMBAD for the first reference.
in source:	NAME LEO GROUP = NAME M 96 GROUP
in source:	NAME DORADO GROUP
in source:	NAME NGC 1400 GROUP
in source:	NAME NGC 5044 GROUP
in source:	NAME Antlia Cluster
Ref:	=1990AJ....100....1F
by	FERGUSON H.C. , SANDAGE A.
	Astron. J., 100, 1-31 (1990)
	Population studies in groups and clusters of galaxies. III. A catalog of galaxies in five nearby groups.
o	Table II: <FSG II-NN> = <[FS90] Leo NN> (Nos 1-52). Table III: <FSG III-NN> = <[FS90] Dorado NN> (Nos 1-79). Table IV: <FSG IV-NNN> = <[FS90] NGC 1400 NNN> (Nos 1-120). Table V: <FSG V-NNN> = <[FS90] NGC 5044 NNN> (Nos 1-162). Table VI: <FSG VI-NNN> = <[FS90] Antlia NNN> (Nos 1-375).
Ref:	=1999A&A...345..403C
by	CELLONE S.A.
	Astron. Astrophys., 345, 403-413 (1999)
	Surface brightness profiles of dwarf galaxies in the NGC 5044 group: a critical revision of the luminosity - shape relation as a distance indicator.
o	Table 1 (galaxies) and Table 3: objects are 'FSG V-NNN'
o	Table 2: <[FS90] NGC 5044 NNNA> (Nos 49A, 83A, 95A).
Ref:	=2005MNRAS.356...41C
by	CELLONE S.A. , BUZZONI A.
	Mon. Not. R. Astron. Soc., 356, 41-53 (2005)
	The low-luminosity galaxy population in the NGC5044 Group.
o	Table 2: <[CB2005] AN> (Nos B1-B4). Table 3: <[FS90] NGC 5044 NNNA> (Nos 54A, 64A, 70A, 93A-93C) added.
=E=	Catalogue in electronic form as VII/180
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FS95]
[FS95]	(Freyberg+Schmitt, 1995)= ([FS95a])
Write:	<<[FS95] NN>>
N:	52
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations. N=52 X-ray sources in the region of NGC 2024.
in source:	NGC 2024
Ref:	=1995A&A...296L..21F
by	FREYBERG M.J. , SCHMITT J.H.M.M.
	Astron. Astrophys., 296, 21-24 (1995)
	ROSAT X-ray observations of the stellar clusters in NGC 2023 and NGC 2024.
o	IRS -> [BCB89], FIR -> [MCK88] NGC 2024, CS -> [SGZ91]
o	Table 1: <[FS95] NN> (Nos 1-52)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FS95a]
[FS95a]	(Freyberg+Schmitt, 1995)
*****	Avoid the usage of [FS95a], prefer [FS95]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FS95b]
[FS95b]	(Fabrika+Sholukhova, 1995)
Write:	<<[FS95b] LNNN-N>> <<[FS95b] HA NN>>
N:	25+20
Object:	OB* + H-alpha (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table II: N=25, format 'LNNN-N', where 2 or 3 stars (LNNN-1, -2, -3) are coinciding with one 'LNNN' = 'LMA M 33 NNN' object. Table VI: N=20 H-alpha em. stars, format 'HA-NNN'. Other formats 'BBNNN-N' in Table III, 'DDBN-N' or 'LgHHMMm+DDMMm-N' in Table IV, are not actually included in SIMBAD.
Ref:	=1995Ap&SS.226..229F
by	FABRIKA S. , SHOLUKHOVA O.
	Astrophys. Space Sci., 226, 229-244 (1995)
	A search for unique objects in nearby galaxies.
o	Tables III, IV: objects ending by '/N' are not in SIMBAD
o	Table II: <[FS95b] LNNN-N> N=25. Table VI: <[FS95b] HA NN> (Nos 1-20)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FS96]
[FS96]	(Fabrika+Sholukhova, 1996)
Write:	<<[FS96] NNN>>
N:	42 among 549
Object:	H-alpha Blue * (SIMBAD class: Star)
Note:	BTA 6m telescope spectroscopy of N=59 blue stars with possible Halpha emission. Table, col(1): numbering 'NNN' is coming from Fabrika + Sholukhova, 1996 catalogue, in 'Bull. Special Astrophys. Obs.' N=42 among 549
in source:	M 33 = NGC 598
Ref:	=1997PAZh...23..524S
by	SHOLUKHOVA O.N. , FABRIKA S.N., VLASYUK V.V., BURENKOV A.N.
	Pis'ma Astron. Zh., 23, 524-531 (1997)
	Spectroscopic observations of Hα-emission blue stars in the galaxy M 33.
o	Table, col(1): <[FS96] NNN> N=42 among 549
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FSA
FSA	(Faint Standard Adaptive Optics) >>>>>> New acronym being registered
Object:	(Near IR) G
Auth.:	SMAIL I.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: FSAO
FSAO	(Faint Standard Adaptive Optics)
Write:	<<FSAO JHHMMSS.ss+DDMMSS.s>>
N:	111
Object:	(Near IR) G (SIMBAD class: Galaxy)
Note:	Catalogue of Potential Adaptive Optics Survey Fields from the UKIRT Archive. See also [CS2006] designations and FS.
Ref:	=2006MNRAS.365..439C
by	CHRISTOPHER N.M. , SMAIL I.
	Mon. Not. R. Astron. Soc., 365, 439-446 (2006)
	A catalogue of potential adaptive optics survey fields from the UKIRT archive.
o	Table 2, col(1): <[CS2006] FSNNN-NN> N=111 = Table 2, col(2): <FSAO JHHMMSS.ss+DDMMSS.s> N=111.
=E=	Catalogue in electronic form as J/MNRAS/365/439
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [FSB2005]
[FSB2005]	(Feretti+Schuecker+Borhringer+, 2005)
Write:	<<[FSB2005] JHHMMSS.s+DDMMSS>> <<[FSB2005] AN>> <<[FSB2005] JHHMMSS.ss+DDMMSS.s>>
N:	2+3+5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Deep VLA observations of 2 clusters: In RXC J0437.1+0043, 2 radio sources are found, format JHHMMSS.s+DDMMSS. In RXC J1314.4-2515, 3 radio sources are found, (Nos H, R1-R2). Source R1 has 3 possible optical identifications, source R2 has 2 possible optical identifications. See also [VMP2002].
in source:	RXC J0437.1+0043 = 1RXS J043709.8+004337
in source:	RXC J1314.4-2515 = 1RXS J131423.6-251521
Ref:	=2005A&A...444..157F
by	FERETTI L. , SCHUECKER P., BOEHRINGER H., GOVONI F., GIOVANNINI G.
	Astron. Astrophys., 444, 157-164 (2005)
	Diffuse radio emission in a REFLEX cluster.
o	Paragraph 2. Calibrator J1284-199 not identified (wrong coordinates)
o	Table 2: <[FSB2005] JHHMMSS.s+DDMMSS> N=2. Table 3, Fig.6: <[FSB2005] AN> (Nos H, R1-R2). Table 3: <[FSB2005] JHHMMSS.ss+DDMMSS.s> N=3+2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSB98]
[FSB98]	(Fischer+Schade+Barrientos, 1998)= (HST)
Write:	<<[FSB98] J1411+5211>> <<[FSB98] J1411+5211 A>> <<[FSB98] J1411+5211 G>>
N:	1+1+4
Object:	Lens (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC observations of ClG 1409+52. quadruple system: The lensing galaxy is [DG92] 6- 162, the lensed galaxy is [FSB98] J1411+5211 G, and 4 images A to D are seen.
in source:	ClG 1409+5226
Ref:	=1998ApJ...503L.127F
by	FISCHER P. , SCHADE D., BARRIENTOS L.F.
	Astrophys. J., 503, 127-130 (1998)
	Discovery of a new quadruple lens HST 1411+5211.
o	Table 1, Fig.1: <[FSB98] J1411+5211> N=1, <[FSB98] J1411+5211 A> (Nos A-D). Text: <[FSB98] J1411+5211 G> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FSC
FSC	(FAUST Catalog)
*****	Avoid the usage of FSC, prefer [BOA98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FSC
FSC	(FAUST Catalog)
Origin	of the Acronym: L (1998MNRAS.295..959B)
Details on Acronym: FSC
FSC	(Faint Source Catalog)
**	catalog: use IRAS
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [FSC2011]
[FSC2011]	(Freudling+Staveley-Smith+Catinella+, 2011)= (AUDS)
Write:	<<[FSC2011] AUDS N-N>>
N:	18
Object:	HI G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=18 HI 21cm line sources detected in a precursor projet for the Arecibo Ultra Deep Survey (AUDS). In format N-N: the first digit is the number of the strip (1, 2 or 3), and the second is a running number within the strip in order of increasing right ascension.
Ref:	=2011ApJ...727...40F
by	FREUDLING W. , STAVELEY-SMITH L., CATINELLA B., MINCHIN R., CALABRETTA M., MOMJIAN E., ZWAAN M., MEYER M., O'NEIL K.
	Astrophys. J., 727, 40 (2011)
	Deep 21 cm H I observations at z ~ 0.1: the precursor to the Arecibo Ultra Deep Survey.
o	Fig. 2, Table 2: <[FSC2011] AUDS N-N> N=18.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSC2019]
[FSC2019]	(Ferreira+Santos+Corradi+, 2019)
Write:	<<[FSC2019] UFMG NN>>
N:	96
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	N=3+62+34 open clusters using Gaia DR2 data.
Ref:	=2019MNRAS.483.5508F
by	FERREIRA F.A. , SANTOS J.F.C., CORRADI W.J.B., MAIA F.F.S., ANGELO M.S.
	Mon. Not. R. Astron. Soc., 483, 5508-5517 (2019)
	Three new Galactic star clusters discovered in the field of the open cluster NGC 5999 with Gaia DR2.
o	Fig. 1, Table 1: <[FSC2019] UFMG N> (Nos UFMG 1-UFMG 3).
Ref:	=2020MNRAS.496.2021F
by	FERREIRA F.A. , CORRADI W.J.B., MAIA F.F.S., ANGELO M.S., SANTOS J.F.C.
	Mon. Not. R. Astron. Soc., 496, 2021-2038 (2020)
	Discovery and astrophysical properties of Galactic open clusters in dense stellar fields using Gaia DR2.
o	param.dat: <[FSC2019] UFMG NN> (Nos 4-62) added.
Ref:	=2021MNRAS.502L..90F
by	FERREIRA F.A. , CORRADI W.J.B., MAIA F.F.S., ANGELO M.S., SANTOS J.F.C.
	Mon. Not. R. Astron. Soc., 502L, 90-94 (2021)
	New star clusters discovered towards the Galactic bulge direction using Gaia DR2.
o	param.dat: <[FSC2019] UFMG NN> (Nos 63-96) added.
=E=	Catalogue in electronic form as <J/MNRAS/483/5508/>
=E=	Catalogue in electronic form as <J/MNRAS/496/2021/>
=E=	Catalogue in electronic form as <J/MNRAS/502/L90/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSE2005]
[FSE2005]	(Froebrich+Scholz+Eisloffel+, 2005)
Write:	<<[FSE2005] NN>>
N:	25
Object:	Globule (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	NIR observations at the 2.2m telescope at Calar Alto. Use of 2MASS archival data. Optical imaging at the 2m telescope at the Thueringer Landessternwarte Tautenburg. Search for young stellar populations in globules.
in source:	IC 1396W
Ref:	=2005A&A...432..575F
by	FROEBRICH D. , SCHOLZ A., EISLOEFFEL J., MURPHY G.C.
	Astron. Astrophys., 432, 575-584 (2005)
	Star formation in globules in IC 1396.
o	Table 1: <[FSE2005] NN> (Nos 1-25).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSF98]
[FSF98]	(Frayer+Seaquist+Frail, 1998)
Write:	<<[FSF98] NN>>
N:	10
Object:	OH Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	Table 1: (Nos 1-10), candidate maser regions (OH feature)
in source:	NGC 253
Ref:	=1998AJ....115..559F
by	FRAYER D.T. , SEAQUIST E.R., FRAIL D.A.
	Astron. J., 115, 559-572 (1998)
	OH satellite-line masers in the nucleus of NGC 253.
o	p.560: calibrators not identified. pp.570-571: UA97 objects = [AU88] S.ss-SS.s, HCN regions 5 and 6 = [PTJ95] 5 and 6, CS complex B = [PZW96] B
o	Table 1: <[FSF98] NN> (Nos 1-10)
Details on Acronym: FSG
FSG	(Ferguson+Sandage, Group)
Write:	<<FSG R-NNN>>
N:	788
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table II: (Nos 1-52), G in Leo group, format 'II-NN'. Table III: (Nos 1-79), G in Dorado group, format 'III-NN'. Table IV: (Nos 1-120), G in NGC 1400 group, format 'IV-NNN'. Table V: (Nos 1-162), G in NGC 5044 group, format 'V-NNN'. Table VI: (Nos 1-375), G in Antlia group, I-NNN'. Also designated as [FS90] in SIMBAD.
in source:	NAME LEO GROUP = NAME M 96 GROUP
in source:	NAME DORADO GROUP
in source:	NAME NGC 1400 GROUP
in source:	NAME NGC 5044 GROUP
in source:	NAME Antlia Cluster
Ref:	=1990AJ....100....1F
by	FERGUSON H.C. , SANDAGE A.
	Astron. J., 100, 1-31 (1990)
	Population studies in groups and clusters of galaxies. III. A catalog of galaxies in five nearby groups.
o	Table II: <FSG II-NN> = <[FS90] Leo NN> (Nos 1-52). Table III: <FSG III-NN> = <[FS90] Dorado NN> (Nos 1-79). Table IV: <FSG IV-NNN> = <[FS90] NGC 1400 NNN> (Nos 1-120). Table V: <FSG V-NNN> = <[FS90] NGC 5044 NNN> (Nos 1-162). Table VI: <FSG VI-NNN> = <[FS90] Antlia NNN> (Nos 1-375).
=E=	Catalogue in electronic form as VII/180
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [FSG2010]
[FSG2010]	(Frebel+Simon+Geha+, 2010)
Write:	<<[FSG2010] UMaII-SN>> <<[FSG2010] UMaII-NM>> <<[FSG2010] ComBer-SN>>
N:	3+1+3
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Keck HIRES observations of Ursa Major II and Coma Berenices.
in source:	NAME UMa II Galaxy
in source:	NAME Coma Dwarf Galaxy
Ref:	=2010ApJ...708..560F
by	FREBEL A. , SIMON J.D., GEHA M., WILLMAN B.
	Astrophys. J., 708, 560-583 (2010)
	High-resolution spectroscopy of extremely metal-poor stars in the least evolved galaxies: Ursa Major II and Coma Berenices.
o	Tables 1-2: <[FSG2010] UMaII-SN> (Nos UMaII-S1 to UMaII-S3), <[FSG2010] UMaII-NM> N=1, <[FSG2010] ComBer-SN> (Nos ComBer-S1 to ComBer-S3).
=E=	Catalogue in electronic form as <J/ApJ/708/560/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSH2003]
[FSH2003]	(Froebrich+Smith+Hodapp+, 2003)= (FIRS)
Write:	<<[FSH2003] HH 211 FIRS N>> <<[FSH2003] IC 1396W FIRS N>> <<[FSH2003] LDN 1211 FIRS N>>
N:	1+2+1
Object:	(Far IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	For-IR photometry with ISO photopolarimeter. Additional sources in HH 211, IC 1396W, and LDN 1211 fields. The numbering is beginning by the number 2, the first sources for authors are already known as HH 211 IR, IC 1396W, and IRAS 22451+6154.
Ref:	=2003MNRAS.346..163F
by	FROEBRICH D. , SMITH M.D., HODAPP K.-W., EISLOEFFEL J.
	Mon. Not. R. Astron. Soc., 346, 163-176 (2003)
	Far-infrared photometry of deeply embedded outflow sources.
o	Table 2: <[FSH2003] HH 211 FIRS N> (No. 2), <[FSH2003] IC 1396W FIRS N> (Nos 2, 3), <[FSH2003] LDN 1211 FIRS N> (No. 2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSH2010]
[FSH2010]	(Forbes+Spitler+Harris+, 2010)
Write:	<<[FSH2010] JHHMMSS.sss+DDMMSS.ss>> <<[FSH2010] JHHMMSS.s+DDMMSS.s>>
N:	142+1
Object:	Poss. GlCl + Poss. UCD (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	HST ACS observations of possible globular clusters in NGC 5170.
in source:	NGC 5170
Ref:	=2010MNRAS.403..429F
by	FORBES D.A. , SPITLER L.R., HARRIS W.E., BAILIN J., STRADER J., BRODIE J.P., LARSEN S.S.
	Mon. Not. R. Astron. Soc., 403, 429-438 (2010)
	A blue tilt in the globular cluster system of the Milky Way-like galaxy NGC 5170.
o	Table 1: <[FSH2010] JHHMMSS.sss+DDMMSS.ss> N=142. Text: <[FSH2010] J132953.4-175909.1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSH2012]
[FSH2012]	(Fotopoulou+Salvato+Hasinger+, 2012)= ([FSH2012a])
Write:	<<[FSH2012] NNNNNN>>
N:	187611
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Large Binocular Telescope (LBT) UBVYz' observations of the Lockman Hole. Use of XMM, GALEX, Subaru, SDSS, UKIDSS and Spitzer data.
in source:	NAME Lockman Hole
Ref:	=2012ApJS..198....1F
by	FOTOPOULOU S. , SALVATO M., HASINGER G., ROVILOS E., BRUSA M., EGAMI E., LUTZ D., BURWITZ V., HENRY J.P., HUANG J.H., RIGOPOULOU D., VACCARI M.
	Astrophys. J., Suppl. Ser., 198, 1 (2012)
	Photometry and photometric redshift catalogs for the Lockman Hole deep field.
o	Tables 5, 10: <[FSH2012] NNNNNN> N=187611 among (Nos 1-206786).
=E=	Catalogue in electronic form as J/ApJS/198/1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSH2012a]
[FSH2012a]	(Fotopoulou+Salvato+Hasinger+, 2012)
*****	Avoid the usage of [FSH2012a], prefer [FSH2012]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSH2012b]
[FSH2012b]	(FRANCK+SHAFTER+HORNOCH+, 2012)
Write:	<<[FSH2012b] N2403 YYYY-NNa>> <<[FSH2012b] N2403-SN>>
N:	9+3
Object:	No? + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	INT WFC and 2.3m Bok telescope narrow-band observations of NGC 2403 in the Halpha line.
in source:	NGC 2403
Ref:	=2012ApJ...760...13F
by	FRANCK J.R. , SHAFTER A.W., HORNOCH K., MISSELT K.A.
	Astrophys. J., 760, 13 (2012)
	The nova rate in NGC 2403.
o	Paragr. 2.2: <[FSH2012b] N2403-SN> (Nos S1-S3), Table 2: <[FSH2012b] N2403 YYYY-NNa> N=9
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSH98]
[FSH98]	(Feldt+Stecklum+Henning+, 1998)
Write:	<<[FSH98] a>> <<[FSH98] aW>> <<[FSH98] R>> <<[FSH98] MIR N>>
N:	14+1+6+2
Object:	(IR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Stat:	is completely incorporated in Simbad
Note:	ESO 3.6m ADONIS NIR and Gemini North NIFS observations of [WC89] 45.45+0.06 region: (Nos a-o, hS), j missing, N=14 sources inside the VLA map. (Nos I to VI), N=6 other point sources in the image. MIR 1 is a strong Mid-IR source, MIR 2 is faintest (text p.763). See also [FSH99]
in source:	[WC89] 045.45+0.06
Ref:	=1998A&A...339..759F
by	FELDT M. , STECKLUM B., HENNING T., HAYWARD T.L., LEHMANN T., KLEIN R.
	Astron. Astrophys., 339, 759-772 (1998)
	The ultracompact H II region G45.45+0.06. A pearl necklace in the sky.
o	T.1 : Y 4338 not identified (PLX?), gam Aqu : Aql or Aqr?, GL 748 : AFGL or GJ?
o	Table 2: <[FSH98] a> (Nos a-o, j missing), <[FSH98] R> (Nos I to VI), <[FSH98] MIR N> (Nos 1-2).
Ref:	=2008AJ....135.1708B
by	BLUM R.D. , McGREGOR P.J.
	Astron. J., 135, 1708-1717 (2008)
	The ionizing stars of the galactic ultra-compact H II region G45.45+0.06.
o	Fig.2: <[FSH98] aW> (No. hS) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSH99]
[FSH99]	(Feldt+Stecklum+Henning+, 1999)
Write:	<<[FSH99] H2 A>> <<[FSH99] NNA>>
N:	3+22
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	NIR photometry at the ESO 2.2m and 3.6m telescopes at La Silla. N=3 regions A to C with measured H2 flux and 5 YSO candidates. See also [FSH98].
in source:	[WC89] 005.89-0.39
Ref:	=1999A&A...346..243F
by	FELDT M. , STECKLUM B., HENNING T., LAUNHARDT R., HAYWARD T.L.
	Astron. Astrophys., 346, 243-259 (1999)
	High-resolution imaging of ultracompact HII regions. II. G5.89-0.39 revisited.
o	:Fig.6: <[FSH99] H2 A> (Nos A-C). Fig.11, Table 3: <[FSH99] NN> (Nos 0-21).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSI2000]
[FSI2000]	(Frayer+Smail+Ivison+, 2000)
Write:	<<[FSI2000] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Note:	N=1 galaxy detected at 1.29 mm by OVRO, counterpart of [SIB98] SMM J00266+1708. This new galaxy seems to be the counterpart of the SMM.
Ref:	=2000AJ....120.1668F
by	FRAYER D.T. , SMAIL I., IVISON R.J., SCOVILLE N.Z.
	Astron. J., 120, 1668-1674 (2000)
	The identification of the submillimeter galaxy SMM J00266+1708.
o	SMM J00266+1708 = [SIB98] SMM J00266+1708. Galaxies M1, M2, M8 = [BCS99b] Cl 0024+16 M1, M2, M8. Galaxies SMM J1401+0252 J1/J2 = [BCS99b] ACO 1835 J1, J2. ERO N4 = [BCS99b] Cl 0440+02 N4.
o	<[FSI2000] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSK2002]
[FSK2002]	(Fujita+Sarazin+Kempner+, 2002)
Write:	<<[FSK2002] A>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of ACO 133: N=3 point sources.
in source:	ACO 133
Ref:	=2002ApJ...575..764F
by	FUJITA Y. , SARAZIN C.L., KEMPNER J.C., RUDNICK L., SLEE O.B., ROY A.L., ANDERNACH H., EHLE M.
	Astrophys. J., 575, 764-778 (2002)
	Chandra observations of the disruption of the cool core in A133.
o	cD galaxy = ESO 541-13
o	Fig.2: <[FSK2002] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSK2007]
[FSK2007]	(Ferrero+Sanchez+Kann+, 2007)
Write:	<<[FSK2007] N>> <<[FSK2007] A>>
N:	7+9
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 observations of GRB 050813.
Ref:	=2007AJ....134.2118F
by	FERRERO P. , SANCHEZ S.F., KANN D.A., KLOSE S., GREINER J., GOROSABEL J., HARTMANN D.H., HENDEN A.A., MOLLER P., PALAZZI E., RAU A., STECKLUM B., CASTRO-TIRADO A.J., FYNBO J.P.U., HJORTH J., JAKOBSSON P., KOUVELIOTOU C., MASETTI N., PIAN E., TANVIR N.R., WIJERS R.A.M.J.
	Astron. J., 134, 2118-2123 (2007)
	Constraints on an optical afterglow and on supernova light following the short burst GRB 050813.
o	Fig.1, Table 2: <[FSK2007] N> (Nos 1-7). Table 3: <[FSK2007] A> (Nos A-I).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSL2005]
[FSL2005]	(Fu+Stockton+Liu, 2005)= (ER) = (IDSCL)
Write:	<<[FSL2005] IDSCL JHHMM+DDMM>> <<[FSL2005] ER JHHMMSS.s+DDMMSS>>
N:	1+9
Object:	Cluster of G + G in ClG (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Institute for Astronomy Deep Survey (IfA-DS, Subaru SuprimeCam observations) with complementary Keck I spectroscopy: Discovery of Extremely Red objects (ER in the format) part of a cluster designated as IDSCL J0749+1018.
in source:	[FSL2005] IDSCL J0749+1018
Ref:	=2005ApJ...632..831F
by	FU H. , STOCKTON A., LIU M.
	Astrophys. J., 632, 831-840 (2005)
	Morphologies in a cluster of extremely red galaxies with old stellar populations at z = 1.34.
o	Text: <[FSL2005] IDSCL JHHMM+DDMM> N=1. Table 1: <[FSL2005] ER JHHMMSS.s+DDMMSS> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSL2006]
[FSL2006]	(Fynbo+Starling+Ledoux+, 2006) (Not yet in Simbad)
Write:	<<[FSL2006] GRB 060206 abs N.NN>>
N:	2
Object:	Absorber
Note:	BAT aboard the Swift satellite observations. See also [FLC2006b] and [HSD2007].
Ref:	=2006A&A...451L..47F
by	FYNBO J.P.U. , STARLING R.L.C., LEDOUX C., WIERSEMA K., THOENE C.C., SOLLERMAN J., JAKOBSSON P., HJORTH J., WATSON D., VREESWIJK P.M., MOLLER P., ROL E., GOROSABEL J., NAERAENEN J., WIJERS R.A.M.J., BJOERNSSON G., CASTRO CERON J.M., CURRAN P., HARTMANN D.H., HOLLAND S.T., JENSEN B.L., LEVAN A.J., LIMOUSIN M., KOUVELIOTOU C., NELEMANS G., PEDERSEN K., PRIDDEY R.S., TANVIR N.R.
	Astron. Astrophys., 451, 47-50 (2006)
	Probing cosmic chemical evolution with γ-ray bursts: GRB 060206 at z = 4.048.
o	Text: <[FSL2006] GRB 060206 abs N.NN> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSM2016]
[FSM2016]	(For+Staveley-Smith+McClure-Griffiths+, 2016)
Write:	<<[FSM2016] HVC LLL.l+BB.b+VVV A>>
N:	2+5+3+2+6
Object:	Clump (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA HI observations of N=2+5+3+2+6 clumps in five high-velocity clouds in the Magellanic Leading Arm region.
in source:	HVC 252.2-20.5+310
in source:	HVC 266.0-18.7+338
in source:	HVC 276.3-09.0+277
in source:	HVC 297.1+08.5+253
in source:	HVC 310.3+08.1+167
Ref:	=2016MNRAS.461..892F
by	FOR B.-Q. , STAVELEY-SMITH L., McCLURE-GRIFFITHS N.M., WESTMEIER T., BEKKI K.
	Mon. Not. R. Astron. Soc., 461, 892-907 (2016)
	The distance and properties of hydrogen clouds in the Leading Arm of the Magellanic System.
o	Fig. 9, Table 2: <[FSM2016] HVC LLL.l+BB.b+VVV A> N=2+5+3+2+6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSM97]
[FSM97]	(Fabbiano+Schweizer+Mackie, 1997)
Write:	<<[FSM97] X-NN>>
N:	16
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations. Table 1: (Nos X-1 to X-12), sources in The Antennae. Table 3: (Nos X-13 to X-16), sources in The Antennae field
in source:	NAME the Antennae
Ref:	=1997ApJ...478..542F
by	FABBIANO G. , SCHWEIZER F., MACKIE G.
	Astrophys. J., 478, 542-553 (1997)
	ROSAT HRI observations of NGC 4038/4039, ``The Antennae'' galaxies.
o	Tables 1, 3: <[FSM97] X-NN> (Nos 1-16)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FSO
FSO	(Flare Star)
Write:	<<FSO BNN>>
N:	32
Object:	Flare * (SIMBAD class: Eruptive* = Eruptive Variable)
Note:	In the format the letter 'B' stands for 'Byurakan obs.'. 1st ref.: (Nos B1-B9), 2nd ref.: (Nos B10-B13). Then, there are missing numbers. 3rd ref.: (Nos B19, B24-B28). Some 'BNN' stars are found in ref. 1988Afz....28..540M, among which Nos B31, B32
in source:	NAME Orion Nebula
Ref:	=1979IBVS.1628....1C
by	CHAVUSHIAN H.S. , MELIKIAN N.D., MIRZOYAN L.V., JANKOVICS I.
	IAU Inform. Bull. Var. Stars, 1628, 1-None (1979)
	Flare stars in Orion.
o	<FSO BN> (Nos B1-B9)
Ref:	=1981Ap.....17..197M
by	MIRZOYAN L.V. , CHAVUSHIAN H.S., MELIKIAN N.D., NATSVLISHVILI R.S., OGANIAN G.B., AMBARIAN V.V., GARIBDZHANIAN A.T.
	Astrophysics, 17, 197-213 (1981)
	Photographic colorimetry of stellar flares in the Pleiades and Orion.
o	Table 3: <Cl* Melotte 22 MCM NN> (Nos 1-32), Table 7: <FSO BNN> (Nos B10-B13)
Ref:	=1983Afz....19..725M
by	MIRZOYAN L.V. , CHAVUSHIAN H.S., MELIKIAN N.D., NATSVLISHVILI R.S., HAMBARIAN V.V., BRUTIAN G.H.
	Astrofizika, 19, 725-737 (1983)
	Photographic colorimetry of stellar flares in the Pleiades and Orion aggregates. II.
o	Table 3: <Cl* Melotte 22 ANON PN> (Nos P1-P4), <FSO BNN> (Nos B19, B24, B25, B28)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: FSO
FSO	(Flare Star)
*****	Avoid the usage of FSO, prefer HPRA
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [FSP2006]
[FSP2006]	(Forbes+Sanchez-Blazquez+Phan+, 2006)
Write:	<<[FSP2006] NGC 1407 ANNN>> <<[FSP2006] NGC 1407 KN-NN>> <<[FSP2006] NGC 1400 WNNN>> <<[FSP2006] NGC 1400 KN-NN>>
N:	903+400+204+74
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	Wide-field Keck telescope imaging (letter K in the format) of the globular cluster system around NGC 1407 and NGC 1400, complemented by HST ACS images of NGC 1407 (letter A in the format), and HST WFPC2 images of NGC 1400 (letter W in the format).
in source:	NGC 1407
in source:	NGC 1400
Ref:	=2006MNRAS.366.1230F
by	FORBES D.A. , SANCHEZ-BLAZQUEZ P., PHAN A.T.T., BRODIE J.P., STRADER J., SPITLER L.
	Mon. Not. R. Astron. Soc., 366, 1230-1242 (2006)
	An imaging study of the globular cluster systems of NGC 1407 and 1400.
o	Table A1: <[FSP2006] NGC 1407 ANNN> (Nos A1-A903). Table A2: <[FSP2006] NGC 407 KN-NN> N=400. Table A3: <[FSP2006] NGC 1400 WNNN> (Nos W1-W204). Table A4: <[FSP2006] NGC 1407 KN-NN> (Nos K5-16 to K5-89).
=E=	Catalogue in electronic form as J/MNRAS/366/1230
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FSR
FSR	(Froebrich+Scholz+Raftery)
*****	Avoid the usage of FSR, prefer [FSR2007]
Origin	of the Acronym: L (2007A&A...472..483B)
Details on Acronym: [FSR2007]
[FSR2007]	(Froebrich+Scholz+Raftery, 2007)= (FSR)
Write:	<<[FSR2007] NNNN>>
N:	1021
Object:	Poss. Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Star density maps from 2MASS are used to obtained a sample of star cluters in the entire Galactic Plane.
Ref:	=2007MNRAS.374..399F
by	FROEBRICH D. , SCHOLZ A., RAFTERY C.L.
	Mon. Not. R. Astron. Soc., 374, 399-408 (2007)
	A systematic survey for infrared star clusters with\|b\| <20° using 2MASS.
o	Cluster Whiting 1: WHI B0200-03 = NAME WHITING 1 in SIMBAD.
o	Tables A1, B1: <[FSR2007] NNNN> N=1021 among (Nos 1-1786).
=E=	Catalogue in electronic form as J/MNRAS/374/399
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSR2011]
[FSR2011]	(Foster+Spitler+Romanowsky+, 2011)
Write:	<<[FSR2011] JHHMMSS.ss+DDMMSS.ss>> <<[FSR2011] GCNNN>> <<[FSR2011] UCDN>>
N:	431+143+3+109
Object:	* + GlCl + UCD + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Subaru Suprime-Cam and Keck DEIMOS observations of NGC 4494.
in source:	NGC 4494
Ref:	=2011MNRAS.415.3393F
by	FOSTER C. , SPITLER L.R., ROMANOWSKY A.J., FORBES D.A., POTA V., BEKKI K., STRADER J., PROCTOR R.N., ARNOLD J.A., BRODIE J.P.
	Mon. Not. R. Astron. Soc., 415, 3393-3416 (2011)
	Global properties of `ordinary ' early-type galaxies: photometry and spectroscopy of stars and globular clusters in NGC 4494.
o	Tables 3-4: <[FSR2011] JHHMMSS.ss+DDMMSS.ss> N=431+143. Table A2: <[FSR2011] UCDN> (Nos 1-3), <[FSR2011] GCNNN> (Nos 1-109).
=E=	Catalogue in electronic form as J/MNRAS/415/3393
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FSS
FSS	(Faint Source Survey)
**	catalog: use IRAS
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [FSS2007]
[FSS2007]	(Frieswijk+Spaans+Shipman+, 2007)
Write:	<<[FSS2007] GLLL.ll+B.bb>> <<[FSS2007] PNN>>
N:	1+10
Object:	Dark Cloud + C18O Core (SIMBAD class: MolCld = Molecular Cloud)
Note:	IRAM 30m C18O(2-1) line observations of the field of NGC 7538.
Ref:	=2007A&A...475..263F
by	FRIESWIJK W.W.F. , SPAANS M., SHIPMAN R.F., TEYSSIER D., HILY-BLANT P.
	Astron. Astrophys., 475, 263-275 (2007)
	Physical characteristics of a dark cloud in an early stage of star formation toward NGC 7538. An outer Galaxy infrared dark cloud?
o	Text: <[FSS2007] GLLL.ll+B.bb> N=1. Fig.4, Table 1: [FSS2007] PNN> (Nos P1-P10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FSS2017]
[FSS2017]	(Fukui+Sano+Sato+, 2017)
Write:	<<[FSS2017] CONNWW>> <<[FSS2017] CO25C>>
N:	7
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	NANTEN telescope 12CO observations of N=7 molecular clouds in the field of RX J0852.0-4622 SNR.
in source:	RX J0852.0-4622
Ref:	=2017ApJ...850...71F
by	FUKUI Y. , SANO H., SATO J., OKAMOTO R., FUKUDA T., YOSHIIKE S., HAYASHI K., TORII K., HAYAKAWA T., ROWELL G., FILIPOVIC M.D., MAXTED N., McCLURE-GRIFFITHS N.M., KAWAMURA A., YAMAMOTO H., OKUDA T., MIZUNO N., TACHIHARA K., ONISHI T., MIZUNO A., OGAWA H.
	Astrophys. J., 850, 71-71 (2017)
	A detailed study of the interstellar protons toward the TeV γ-ray SNR RX J0852.0-4622 G266.2-1.2, Vela Jr.): the third case of the γ-ray and ISM spatial correspondence.
o	Table 1: <[FSS2017] CONNWW> N=6, <[FSS2017] CO25C> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FST86]
[FST86]	(Fukui+Sugitani+Takaba+, 1986)
Write:	<<[FST86] Ori A W>> <<[FST86] LDN 1641 WN>> <<[FST86] rho Oph W>> <<[FST86] S140 W>> <<[FST86] NGC 2071 W>>
N:	2+9+1+1+1
Object:	Molecular Outflow (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
in source:	NAME Ori A
in source:	Orion Nebula:LDN 1641 = LDN 1641
in source:	NAME rho Oph Cloud
in source:	SH 2-140
in source:	NGC 2071
Ref:	=1986ApJ...311L..85F
by	FUKUI Y. , SUGITANI K., TAKABA H., IWATA T., MIZUNO A., OGAWA H., KAWABATA K.
	Astrophys. J., 311, 85-88 (1986)
	Discovery of seven bipolar outflows by an unbiased survey.
o	Table 1 : IRAS 22175+6317 misprint for 22178+6317.
o	Table 1: <[FST86] Ori A W> (Nos E, W), <[FST86] LDN 1641 W> (Nos N, S), <[FST86] ρ Oph W> (No. E), <[FST86] S140 W> (No. N), <[FST86] NGC 2071 W> (No. N).
Ref:	=1988VA.....31..217F
by	FUKUI Y.
	Vistas in Astronomy, 31, 217-226 (1988)
	An unbiased survey of star formation regions with the Nagoya 4m radio telescope.
o	Table 1: <[FST86] LDN 1641 WN> (Nos C, S2) added.
Ref:	=1989Natur.342..161F
by	FUKUI Y. , IWATA T., TAKABA H., MIZUNO A., OGAWA H., KAWABATA K., SUGITANI K.
	Nature, 342, 161-163 (1989)
	Molecular outflows in protostellar evolution.
o	Table 1: <[FST86] LDN 1641 WN> (Nos S3, S4) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FST98]
[FST98]	(Fender+Southwell+Tzioumis, 1998)
Write:	<<[FST98] HHMM+DDdW>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Fig.1: Radio map on optical location of the blackhole LMC X-1, with 3 nearby sources.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1998MNRAS.298..692F
by	FENDER R.P. , SOUTHWELL K., TZIOUMIS A.K.
	Mon. Not. R. Astron. Soc., 298, 692-696 (1998)
	A radio survey of supersoft, persistent and transient X-ray sources in the Magellanic Clouds.
o	Fig.1: <[FST98] HHMM-DDdW> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FSTW
FSTW	(Feast+Stoy+Thackeray+Wesselink) (Not yet in Simbad)
Write:	<<FSTW NNN>>
N:	248
Object:	* (SIMBAD class: Star)
Ref:	=1961MNRAS.122..239F
by	FEAST M.W. , STOY R.H., THACKERAY A.D., WESSELINK A.J.
	Mon. Not. R. Astron. Soc., 122, 239-253 (1961)
	Spectral classification and photometry of Southern B stars.
o	Table I: <FSTW NNN> (Nos 1-248).
Origin	of the Acronym: L (1969AJ.....74..882W)
Details on Acronym: FSVS
FSVS	(Faint Sky Variability Survey)
Write:	<<FSVS JHHMM+DDMM>>
N:	13
Object:	Poss. Catacl. V* (SIMBAD class: Variable* = Variable Star)
Note:	2002A&A...395L..47H: First reference with object from the FSVS. See also [HMH2002]
Ref:	=2002A&A...395L..47H
by	HOWELL S.B. , MASON E., HUBER M., CLOWES R.
	Astron. Astrophys., 395, 47-50 (2002)
	Discovery of two new faint cataclysmic variables.
o	The two new CV* are [HMH2002] HA J0242-2802 and FSVS J1722+2723.
o	Table 1: <FSVS JHHMM+DDMM> N=13. Table 1: <[HMH2002] HA JHHMM+DDMM> N=12.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FSVS-CL
FSVS-CL	(Faint Sky Variability Survey, Cluster)
Write:	<<FSVS-CL JHHMMSS+DDMMSS>>
N:	598
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	N=598 galaxy clusters or rich groups discovered in the Faint Sky Variability Survey (FSVS).
Ref:	=2006MNRAS.369.1334S
by	SOCHTING I.K. , HUBER M.E., CLOWES R.G., HOWELL S.B.
	Mon. Not. R. Astron. Soc., 369, 1334-1350 (2006)
	The FSVS Cluster Catalogue: galaxy clusters and groups in the Faint Sky Variability Survey.
o	In table 3 : GHO 2155+0321 not identified, could be a misprint for GHO 215451+023124?
o	Table 4: <FSVS-CL JHHMMSS+DDMMSS> N=598.
=E=	Catalogue in electronic form as J/MNRAS/369/1334
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FSW
FSW	(Freeland+Stilp+Wilcots)
Write:	<<FSW JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Note:	VLA HI line observations of the USGC U070 group of galaxies. Use of DSS optical data.
in source:	USGC U070
Ref:	=2009AJ....138..295F
by	FREELAND E. , STILP A., WILCOTS E.
	Astron. J., 138, 295-304 (2009)
	H I observations of five groups of galaxies.
o	<FSW J014526.92+043619.1> N=1.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: FSZ
FSZ	(Fabrika+Sholukhova+Zakharova)
Write:	<<FSZ NNN>>
N:	549
Object:	Blue * (SIMBAD class: Star)
Note:	The same objects are also published in 1999A&AS..140..309F
in source:	M 33 = NGC 598
Ref:	=1997BSAO...43..133F
by	FABRIKA S.N. , SHOLUKHOVA O.N., ZAKHAROVA S.A.
	Bull. Special Astrophys. Obs., 43, 133-148 (1997)
	Photometry of OB stars on H-α images of M33.
o	objects FSZ are also published in 1999A&AS..140..309F Table 1.
o	Table 1: <FSZ NNN> (Nos 1-549)
=E=	Catalogue in electronic form as <J/A+AS/140/309/>
Origin	of the Acronym: L (1997BSAO...43..149F)
Details on Acronym: [FSZ2014]
[FSZ2014]	(Faherty+Shara+Zurek+, 2014)
Write:	<<[FSZ2014] WR1343-193E>> <<[FSZ2014] WRNNNN-ANN>> <<[FSZ2014] WR1361-1583>> <<[FSZ2014] WR1327-14AF>> <<[FSZ2014] WR1373-1FBA>>
N:	7
Object:	WR (SIMBAD class: WolfRayet* = Wolf-Rayet)
Stat:	is completely incorporated in Simbad
Note:	ITRF SpeX spectroscopy of N=7 Wolf-Rayet stars. Use of WISE and 2MASS data. See also [SMG2009], [SFZ2012], [KSF2015], and [KSF2017].
Ref:	=2014AJ....147..115F
by	FAHERTY J.K. , SHARA M.M., ZUREK D., KANAREK G., MOFFAT A.F.J.
	Astron. J., 147, 115 (2014)
	Characterizing Wolf-Rayet stars in the near- and mid-infrared.
o	Table 5: <[FSZ2014] WR1343-193E> N=1, <[FSZ2014] WRNNNN-ANN> N=3, <[FSZ2014] WR1361-1583> N=1, <[FSZ2014] WR1327-14AF> N=1, <[FSZ2014] WR1373-1FBA> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FT84]
[FT84]	(Fabbiano+Trinchieri, 1984)= (E) = (X)
Write:	<<[FT84] N>>
N:	8
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Einstein HRI observations. Map in Fig. 1. See also: [FT87], [F88], [TFP88], [TFR90], TF, [FKT92]
in source:	NGC 253
Ref:	=1984ApJ...286..491F
by	FABBIANO G. , TRINCHIERI G.
	Astrophys. J., 286, 491-497 (1984)
	The complex X-emission of NGC 253.
o	Table 1: <[FT84] N> (Nos 1-8)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FT87]
[FT87]	(Fabbiano+Trinchieri, 1987)
Write:	<<[FT87] IC 342 N>> <<[FT87] NGC 2403 N>> <<[FT87] NGC 6946 N>>
N:	5+5+2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Einstein satellite observations. Map in Fig. 1. See also: [FT84], [F88], [TFP88], [TFR90], TF, [FKT92]
in source:	IC 342
in source:	NGC 2403
in source:	NGC 6946
Ref:	=1987ApJ...315...46F
by	FABBIANO G. , TRINCHIERI G.
	Astrophys. J., 315, 46-67 (1987)
	X-ray observations of spiral galaxies. II. Images and spectral parameters of 13 galaxies.
o	Table 3: <[FT87] IC 342 N> (Nos 1-5), <[FT87] NGC 2403 N> (Nos 1-5), <[FT87] NGC 6946 N> (Nos 1-2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FT96]
[FT96]	(Fich+Terebey, 1996)= ([FT96a])
Write:	<<[FT96] LLL.l+B.b>> <<[FT96] LLL.l+B.bA>>
N:	109+90
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Table 2: N=109 sources 'LLL.l+B.b'. Table 3: N=90 part of complex sources 'LLL.l+B.bA'
Ref:	=1996ApJ...472..624F
by	FICH M. , TEREBEY S.
	Astrophys. J., 472, 624-642 (1996)
	IRAS observations of the outer Galaxy. I. Discrete sources and large-scale (diffuse) emission.
o	Table 2: <[FT96] LLL.l+B.b> N=109. Table 3: <[FT96] LLL.l+B.bA> N=90
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FT96a]
[FT96a]	(Fich+Terebey, 1996)
*****	Avoid the usage of [FT96a], prefer [FT96]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FT96b]
[FT96b]	(Fiorucci+Tosti, 1996)
Write:	<<[FT96b] 3C 66A CN>> <<[FT96b] PKS HHMM+DDd CN>> <<[FT96b] OJ 287 CN>> <<[FT96b] B2 HHMM+DD CN>> <<[FT96b] ON 231 CN>> <<[FT96b] Mkn 501 CN>> <<[FT96b] H 1722+119 CN>>
N:	30
Object:	* (SIMBAD class: Star)
Note:	N=30 comparison stars 'CN' in the fields of 10 BL Lac objects. See also Paper II: [FTR98]. Finding charts.
Ref:	=1996A&AS..116..403F
by	FIORUCCI M. , TOSTI G.
	Astron. Astrophys., Suppl. Ser., 116, 403-407 (1996)
	VRI photometry of stars in the fields of 12 BL Lacertae objects.
o	Stars with formats 'A' and 'NN' are from other lists: [KC71], [W73], [CJT75], [SJE91], [BDV69] (format 'a', not 'A'). in ref list read Von Montigny for Von Montagny
o	Table 3: <[FT96b] 3C 66A CN>, <[FT96b] PKS HHMM+DDd CN>, <[FT96b] OJ 287 CN>, <[FT96b] B2 HHMM+DD CN>, <[FT96b] ON 231 CN>, <[FT96b] Mkn 501 CN>, <[FT96b] H 1722+119 CN>, N=30.
=E=	Catalogue in electronic form as J/A+AS/116/403
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FTB2000]
[FTB2000]	(Foster+Theissen+Butler+, 2000)
Write:	<<[FTB2000] JHHMMSS.ss+DDMMSS.s>>
N:	634+4078
Object:	* in Cl* (SIMBAD class: Star)
Note:	Table 5: N=634 stars members of Cl Stock 2. Appendix: complete list of CCD photometry.
in source:	Cl Stock 2
Ref:	=2000A&AS..143..409F
by	FOSTER D.C. , THEISSEN A., BUTLER C.J., ROLLESTON W.R.J., BYRNE P.B., HAWLEY S.L.
	Astron. Astrophys., Suppl. Ser., 143, 409-420 (2000)
	CCD photometry and proper motions of late-type stars in the young open cluster Stock 2.
o	Table 5: <[FTB2000] JHHMMSS.ss+DDMMSS.s> N=634. Appendix: <[FTB2000] JHHMMSS.ss+DDMMSS.s> N=4078.
=E=	Catalogue in electronic form as J/A+AS/143/409
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FTBW
FTBW	(Frogel+Terndrup+Blanco+Whitford)
====>	Equivalent to: TFW
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FTC2003]
[FTC2003]	(Fiaschi+Tiveron+Cardullo, 2003)
Write:	<<[FTC2003] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Note:	Astronomical Observatory G. Colombo observations. Discovery of a new nova in M 31.
in source:	M 31 = NGC 224 3H S
Ref:	=2003IAUC.8226....2F
by	FIASCHI M. , TIVERON D., CARDULLO A.
	IAU Circ., 8226, 2-None (2003)
	Nova in M31.
o	<[FTC2003] JHHMMSS.ss+DDMMSS.s> N=1.
Details on Acronym: [FTC2015]
[FTC2015]	(Finoguenov+Tanaka+Cooper+, 2015)
Write:	<<[FTC2015] NN>>
N:	46
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	Detection of N=46 X-ray galaxy groups detected in the Extended Chandra Deep Field South field (ECDF-S). Use of archival Chandra and XMM data.
in source:	NAME Extended Chandra Deep Field South
Ref:	=2015A&A...576A.130F
by	FINOGUENOV A. , TANAKA M., COOPER M., ALLEVATO V., CAPPELLUTI N., CHOI A., HEYMANS C., BAUER F.E., ZIPARO F., RANALLI P., SILVERMAN J., BRANDT W.N., XUE Y.Q., MULCHAEY J., HOWES L., SCHMID C., WILMAN D., COMASTRI A., HASINGER G., MAINIERI V., LUO B., TOZZI P., ROSATI P., CAPAK P., POPESSO P.
	Astron. Astrophys., 576A, 130-130 (2015)
	Ultra-deep catalog of X-ray groups in the Extended Chandra Deep Field-South.
o	Table 4: <[FTC2015] NN> N=46 among (Nos 1-79).
=E=	Catalogue in electronic form as J/A+A/576/A130
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FTC93]
[FTC93]	(Felli+Taylor+Catarzi+, 1993)= (FTCCK)
Write:	<<[FTC93] HHMMSS.ss+DDMMSS.ss>>
N:	7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 5: 7 new compact sources in Orion. (Tables 1, 2: GMR sources). The authors don't give any format to their list, so we use the coordinates as format.
in source:	NAME Orion Nebula
Ref:	=1993A&AS..101..127F
by	FELLI M. , TAYLOR G.B., CATARZI M., CHURCHWELL E., KURTZ S.
	Astron. Astrophys., Suppl. Ser., 101, 127-151 (1993)
	The Orion radio zoo revisited: source variability.
o	Table 1: <GMR NN> (Nos 19-26) added, <GMR A> (Nos L-R) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FTC95]
[FTC95]	(Flin+Trevese+Cirimele+, 1995)
Write:	<<[FTC95] ACO NNNN NNN>>
N:	1167
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Tables 2-11: N=1167 G in 10 ACO clusters. See also [TFM92], [TCC97]
in source:	ACO 151
in source:	ACO 637
in source:	ACO 646
in source:	ACO 649
in source:	ACO 655
in source:	ACO 1132
in source:	ACO 1314
in source:	ACO 1377
in source:	ACO 1570
in source:	ACO 1589
Ref:	=1995A&AS..110..313F
by	FLIN P. , TREVESE D., CIRIMELE G., HICKSON P.
	Astron. Astrophys., Suppl. Ser., 110, 313-327 (1995)
	Properties of nearby clusters of galaxies. II. A 151, A 637, A 646, A 649, A 655, A 1132, A 1314, A 1377, A 1570, A 1589.
o	Tables 2 to 11: <[FTC95] ACO NNNN NNN> N=164+57+235+45+229+62+103+90+69+113
=E=	Catalogue in electronic form as J/A+AS/110/313
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FTCCK
FTCCK	(Felli+Taylor+Catarzi+Churchwell+Kurtz)
*****	Avoid the usage of FTCCK, prefer [FTC93]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FTCCK
FTCCK	(Felli+Taylor+Catarzi+Churchwell+Kurtz)
Note:	The authors' initials in the third ref., Tables 1, 2
*****	Avoid the usage of FTCCK, prefer GMR
Origin	of the Acronym: L = Found in the literature
Details on Acronym: FTHP
FTHP	(Felli+Tofani+Harten+Panagia)
Write:	<<FTHP NN>> <<FTHP Ridge A>>
N:	28+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=28 radio-sources in the field of Sh 2-155, and N=2 ridges.
in source:	SH 2-155
Ref:	=1978A&A....69..199F
by	FELLI M. , TOFANI G., HARTEN R.H., PANAGIA N.
	Astron. Astrophys., 69, 199-211 (1978)
	The thermal radio emission from the S155 nebula and the Cepheus OB 3 association.
o	Table 2: <FTHP NN> (Nos 1-28). Fig.1: <FTHP Ridge A> (Nos A-B).
Origin	of the Acronym: L (1993A&A...273..619M)
Details on Acronym: [FTI2009]
[FTI2009]	(Fraternali+Tolstoy+Irwin+, 2009)
Write:	<<[FTI2009] NN>>
N:	23
Object:	RGB* (SIMBAD class: RGB* = Red Giant Branch star)
Note:	VLT FORS2 spectroscopy of a sample of red giant branch stars in and around the Tucana dwarf galaxy.
in source:	NAME Tucana Dwarf Galaxy
Ref:	=2009A&A...499..121F
by	FRATERNALI F. , TOLSTOY E., IRWIN M.J., COLE A.A.
	Astron. Astrophys., 499, 121-128 (2009)
	Life at the periphery of the local group: the kinematics of the Tucana dwarf galaxy.
o	Table 3: <[FTI2009] NN> (Nos 1-23).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FTI2011]
[FTI2011]	(Freeland+Tran+Irwin+, 2011)
Write:	<<[FTI2011] SN>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT FLAMES/GIRAFFE observations of N=3 disk-dominated galaxies in [GTC2005] SG J1120-1202.
in source:	[GTC2005] SG J1120-1202
Ref:	=2011ApJ...742L..34F
by	FREELAND E. , TRAN K.-V.H., IRWIN T., GIORDANO L., SAINTONGE A., GONZALEZ A.H., ZARITSKY D., JUST D.
	Astrophys. J., 742L, 34 (2011)
	Detection of outflowing and extraplanar gas in disks in an assembling galaxy cluster at z = 0.37.
o	Figs 1+3, Table 1: <[FTI2011] SN> (Nos S1-S3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FTK2009]
[FTK2009]	(Fujishita+Torii+Kudo+, 2009) (Not yet in Simbad)
Write:	<<[FTK2009] MGC 355.5-0.7>>
N:	1
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	NANTEN 12CO and 13CO observations towards the Galactic Center.
in source:	NAME Galactic Center
Ref:	=2009PASJ...61.1039F
by	FUJISHITA M. , TORII K., KUDO N., KAWASE T., YAMAMOTO H., KAWAMURA A., MIZUNO N., ONISHI T., MIZUNO A., MACHIDA M., TAKAHASHI K., NOZAWA S., MATSUMOTO R., FUKUI Y.
	PASJ, 61, 1039-1053 (2009)
	Discovery of molecular loop 3 in the Galactic Center: Evidence for a positive-velocity magnetically floated loop towards L = 355°–359°.
o	Text: <[FYF2006] loop N> (No. 3) added. Table 1: <[FTK2009] MGC 355.5-0.7>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FTM2000]
[FTM2000]	(Fynbo+Thomsen+Moller, 2000)
Write:	<<[FTM2000] gN>> <<[FTM2000] SNNA>>
N:	2+9
Object:	G (SIMBAD class: Galaxy)
Note:	Study of the field around QSO 1205-30. Maps Figs 2-5, 7: N=2 faint galaxies blended with QSO 1205-30 (Nos g1-g2). N=7 sources (Nos S6-S12), S6 being divided into (Nos 6A-6B), S6 is an extended object, S7 to S12 are candidate Lyman-alpha emitting galaxies. The authors used the same numbering (Nos S1-S12) in 3 papers: (Nos S1-S3) are '[MW93] SN', in the field of QSO 0528-250. (Nos S4-S5) are '[FMW99] SN', in the field of QSO 0151+048. (Nos S6-S13) are '[FTM2000] SNN', in the field of QSO 1205-30. See also [MW93], [FMW99].
Ref:	=2000A&A...353..457F
by	FYNBO J.U. , THOMSEN B., MOLLER P.
	Astron. Astrophys., 353, 457-464 (2000)
	Lyα emission from a Lyman limit absorber at z=3.036.
o	Tables 3-4: <[FTM2000] gN> (Nos g1-g2), <[FTM2000] SNNA> (Nos S6-S12, S6A-S6B).
Ref:	=2001A&A...372L..57M
by	MOLLER P. , FYNBO J.U.
	Astron. Astrophys., 372, 57-60 (2001)
	Detection of a redshift 3.04 filament.
o	Table 1: <[FTM2000] SNN> (No. 13) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FTM2003]
[FTM2003]	(Fiaschi+Tiveron+Milani, 2003)
Write:	<<[FTM2003] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Stat:	is completely incorporated in Simbad
Note:	Astronomical Observatory G. Colombo observations. Discovery of a new nova in M 31.
in source:	M 31 = NGC 224
Ref:	=2003IAUC.8253....3F
by	FIASCHI M. , TIVERON D., MILANI L.
	IAU Circ., 8253, 3-None (2003)
	Novae in M31.
o	(Erratum) + corrigendum in IAUC 8254
o	<[FTM2003] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FTR98]
[FTR98]	(Fiorucci+Tosti+Rizzi, 1998)
Write:	<<[FTR98] HHMM+DDd CN>>
N:	44
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=44 comparison stars 'CN' in the fields of 14 Blazars. See also Paper I: [FT96b]. Finding charts.
Ref:	=1998PASP..110..105F
by	FIORUCCI M. , TOSTI G., RIZZI N.
	Publ. Astron. Soc. Pac., 110, 105-110 (1998)
	VRI photometry of stars in the fields of 16 blazars.
o	Table 2: stars with formats 'A' or 'N' are from previously existing lists : [MMW76], [SJE91], [MMM83], PPS, [VRG97], [A71], [CJT75].
o	Table 2: <[FTR98] HHMM+DDd CN> N=44.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FTS2019]
[FTS2019]	(Fukui+Tokuda+Saigo+, 2019) (Not yet in Simbad)
Write:	<<[FTS2019] N159E MMS-N>>
N:	2
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	ALMA Band 6 (211–275 GHz) observations of N=2 millimeter sources toward the N159E-Papillon region. See also [TFH2019].
in source:	Magellanic Clouds:LMC:LHA 120-N 159W = LHA 120-N 159W
Ref:	=2019ApJ...886...14F
by	FUKUI Y. , TOKUDA K., SAIGO K., HARADA R., TACHIHARA K., TSUGE K., INOUE T., TORII K., NISHIMURA A., ZAHORECZ S., NAYAK O., MEIXNER M., MINAMIDANI T., KAWAMURA A., MIZUNO N., INDEBETOUW R., SEWILO M., MADDEN S., GALAMETZ M., LEBOUTEILLER V., CHEN C.-H.R., ONISHI T.
	Astrophys. J., 886, 14-14 (2019)
	An ALMA view of molecular filaments in the Large Magellanic Cloud. I. The formation of high-mass stars and pillars in the N159E-Papillon Nebula triggered by a cloud-cloud collision.
o	Fig. 1: <[FTS2019] N159E MMS-N> (Nos MMS-1 to MMS-2).
o	MMS-1 and MMS-2 are not in SIMBAD.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FTT
FTT	(Falomo+Tanzi+Treves)
*****	Avoid the usage of FTT, prefer [FTT91]
Origin	of the Acronym: L (1993AJ....105.2031F)
Details on Acronym: [FTT91]
[FTT91]	(Falomo+Tanzi+Treves, 1991)= (FTT)
Write:	<<[FTT91] AN>>
N:	7+12
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	NTT and Kitt Peak 4m telescope observations. Pair of Galaxies (Nos A-F), Galaxies in pairs (Nos 'AN'), and Galaxies in the field of the BL Lac object H 0414+00. See also [MLG92].
Ref:	=1991A&A...249..341F
by	FALOMO R. , TANZI E.G., TREVES A.
	Astron. Astrophys., 249, 341-343 (1991)
	A peculiar group of galaxies in the field of the BL Lacertae object H 0414+00.
o	Fig.2, Table 1: <[FTT91] AN> (Nos A-E, A1-A2, B1-B2, C1-C2, D1-D2, E1-E2).
Ref:	=1992MNRAS.256..655M
by	McHARDY I.M. , LUPPINO G.A., GEORGE I.M., ABRAHAM R.G., COOKE B.A.
	Mon. Not. R. Astron. Soc., 256, 655-668 (1992)
	H 0414+009 - an X-ray bright BL Lac with a radio tail in a distant cluster of galaxies.
o	Table 4a: <[MLG92] Object NNNa> (Nos 1-108, 65a). Table 4b: <[MLG92] Star NN> (Nos 1-15). Table 5: <[FTT91] AN> (Nos F-H, F1-F2) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FTV97]
[FTV97]	(Felli+Testi+Valdettaro+, 1997)
Write:	<<[FTV97] MN>> <<[FTV97] S235A*>>
N:	6
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	(Nos M1-M3) 3 IR sources in Sh 2-235 complex, (Nos S235A, S235B, S235C*) 3 stars in Sh 2-235 complex. Maps in Fig. 2 and 7
Ref:	=1997A&A...320..594F
by	FELLI M. , TESTI L., VALDETTARO R., WANG J.-J.
	Astron. Astrophys., 320, 594-604 (1997)
	Star formation in the S 235 A-B complex.
o	Maser in Fig. 2 = [BE83] Maser 173.72+02.70
o	Table 3: <[FTV97] MN> (Nos M1-M3), <[FTV97] S235A> (Nos S235A, S235B, S235C)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FTW2016]
[FTW2016]	(Feher+Toth+Ward-Thompson+, 2016)
Write:	<<[FTW2016] TMC-1FN>>
N:	4
Object:	Core (SIMBAD class: denseCore = Dense Core)
Note:	Effelsberg 100m telescope NH3 line and Herschel SPIRE observations of N=4 sub-filaments of Taurus molecular cloud-1 (TMC-1).
in source:	TMC-1
Ref:	=2016A&A...590A..75F
by	FEHER O. , TOTH L.V., WARD-THOMPSON D., KIRK J., KRAUS A., PELKONEN V.-M., PINTER S., ZAHORECZ S.
	Astron. Astrophys., 590A, 75-75 (2016)
	Structure and stability in TMC-1: Analysis of NH_{3} molecular line and Herschel continuum data.
o	Tables 4-5, Fig.6 :<[FTW2016] TMC-1FN> (Nos 1F1-1F4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Fuen
Fuen	(Fuenmayor, Carbon *)= (FJF) = (FuenC) = (Fuenmayor)
Write:	<<Fuen C NNN>>
N:	283
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-216): in the direction of the Galactic Anticenter. (Nos 217 -283): in the direction of the Galactic Center. Photometry of 211 Fuenmayor's stars in 1989ApJ...336..924J.
Ref:	=1981RMxAA...6...83F
by	FUENMAYOR F.J.
	Rev. Mex. Astron. Astrofis., 6, 83-93 (1981)
	A deep near infrared objective prism survey for carbon stars toward the Galactic Center and Anticenter.
o	in ref list Kurtanidze 1980A&AS...39...35K instead of 89.35
o	Table 1: <Fuen C NNN> (Nos 1-283>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: FuenC
FuenC	(Fuenmayor, Carbon *)
*****	Avoid the usage of FuenC, prefer Fuen
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Fuenmayor
Fuenmayor	(Fuenmayor)
*****	Avoid the usage of Fuenmayor, prefer Fuen
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Furuhjelm
Furuhjelm	(Furuhjelm)
Write:	<<Furuhjelm I-NNNN>> <<Furuhjelm II-NNNN>> <<Furuhjelm III-NNNN>>
N:	1016+1359+1818
Object:	* (SIMBAD class: Star)
Note:	1st ref.: Format 'I-NNNN', N=1016. 2nd ref.: Format 'II-NNNN', N=1359. 3rd ref.: Format 'III-NNNN', N=1818.
Ref:	=1916ASSF...48a...3F
by	FURUHJELM R.
	Acta Soc. Sci. Fennicae, 48, part no 1, 3-185 (1916)
	Recherche sur les mouvements propres des etoiles dans la zone photographique de Helsingfors. I. Cliches de 9h a 12h.
o	<Furuhjelm I-NNNN> (Nos 1-1016)
Ref:	=1926ASSF...50g...3F
by	FURUHJELM R.
	Acta Soc. Sci. Fennicae, 50, part no 7, 3-161 (1926)
	Recherche sur les mouvements propres des etoiles dans la zone photographique de Helsingfors. II. Cliches de 6h a 9h.
o	<Furuhjelm II-NNNN> (Nos 1-1359)
Ref:	=1947ASSFA...3l...3F
by	FURUHJELM R.
	Acta Soc. Sci. Fennicae, Nov. Ser. A, 3, part no 12, 3-90 (1947)
	Recherche sur les mouvements propres des etoiles dans la zone photographique de Helsingfors. III. Cliches de 3h a 6h.
o	<Furuhjelm III-NNNN> (Nos 1-1818)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: FUSE
FUSE	(Far UV Spectroscopic Explorer) (Not yet in Simbad)
Write:	<<FUSE ANNNNNNN>> <<FUSE ANNN-NN>>
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	FUSE internal numbering. First references with this numbering.
Ref:	=2002ApJS..141..443W
by	WALBORN N.R. , FULLERTON A.W., CROWTHER P.A., BIANCHI L., HUTCHINGS J.B., PELLERIN A., SONNEBORN G., WILLIS A.J.
	Astrophys. J., Suppl. Ser., 141, 443-468 (2002)
	Far Ultraviolet Spectroscopic Explorer atlas of OB stars in the Magellanic clouds.
o	Table 1: <FUSE ANNNNNNN> N=56.
Ref:	=2003ApJS..144...21R
by	ROBERT C. , PELLERIN A., ALOISI A., LEITHERER C., HOOPES C., HECKMAN T.M.
	Astrophys. J., Suppl. Ser., 144, 21-45 (2003)
	Synthetic high-resolution line spectra of star-forming galaxies below 1200 Å.
o	Tables 1, 2: <FUSE ANNNNNNN> N=155+85.
Ref:	=2005ApJ...625..167S
by	SOFIA U.J. , WOLFF M.J., RACHFORD B., GORDON K.D., CLAYTON G.C., CARTLEDGE S.I.B., MARTIN P.G., DRAINE B.T., MATHIS J.S., SNOW T.P., WHITTET D.C.B.
	Astrophys. J., 625, 167-180 (2005)
	FUSE measurements of far-ultraviolet extinction. I. Galactic sight lines.
o	<FUSE ANNNNNNN> N=17.
=E=	Catalogue in electronic form as J/ApJS/144/21
=E=	Catalogue in electronic form as B/fuse
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FVD2009]
[FVD2009]	(Foreman+Volonteri+Dotti+, 2009)
Write:	<<[FVD2009] SDSS JHHMM+DDMM>> <<[FVD2009] 2QZ JHHMM+DDMM>>
N:	85
Object:	Pair of QSOs (SIMBAD class: PairG = Pair of Galaxies)
Note:	N=85 pairs of quasars, selected from the SDSS.
Ref:	=2009ApJ...693.1554F
by	FOREMAN G. , VOLONTERI M., DOTTI M.
	Astrophys. J., 693, 1554-1562 (2009)
	Double quasars: probes of black hole scaling relationships and merger scenarios.
o	Table 1: <[FVD2009] SDSS JHHMM+DDMM>, <[FVD2009] 2QZ JHHMM+DDMM>, N=85.
=E=	Catalogue in electronic form as <J/ApJ/693/1554/>
Details on Acronym: [FVD2017]
[FVD2017]	(Farina+Venemans+Decarli+, 2017)
Write:	<<[FVD2017] LAE>>
N:	1
Object:	LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT MUSE observations of N=1 Lyα emitter (LAE) in the field of the QSO J0305−3150.
Ref:	=2017ApJ...848...78F
by	FARINA E.P. , VENEMANS B.P., DECARLI R., HENNAWI J.F., WALTER F., BANADOS E., MAZZUCCHELLI C., CANTALUPO S., ARRIGONI-BATTAIA F., McGREER I.D.
	Astrophys. J., 848, 78-78 (2017)
	Mapping the Lyα emission around a z ~ 6.6 QSO with MUSE: extended emission and a companion at a close separation.
o	Fig. 1, Section 4: <[FVD2017] LAE> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FVK2012]
[FVK2012]	(Fang+van Boekel+King+, 2012)
Write:	<<[FVK2012] CS NN cluster>> <<[FVK2012] N>>
N:	5+3
Object:	Cluster of * + Proplyd (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	N=2 young clusters in the NGC 6357 complex. N=5 proplyds in Cl Pismis 24. Use of 2MASS and GLIMPSE data, and of HST archival images.
in source:	NGC 6357
in source:	Cl Pismis 24
Ref:	=2012A&A...539A.119F
by	FANG M. , VAN BOEKEL R., KING R.R., HENNING T., BOUWMAN J., DOI Y., OKAMOTO Y.K., ROCCATAGLIATA V., SICILIA-AGUILAR A.
	Astron. Astrophys., 539A, 119-119 (2012)
	Star formation and disk properties in Pismis 24.
o	Figs 13-14, Paragr. 3.2.4: <[FVK2012] N> (Nos 1-5). Paragr. 3.1.2: <[FVK2012] CS NN cluster> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FVM2015]
[FVM2015]	(Fernandez-Trincado+Vivas+Mateu+, 2015)
Write:	<<[FVM2015] NN>>
N:	48+2
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Stat:	is completely incorporated in Simbad
Note:	Llano del Hato 1.0m J??rgen Stock telescope QUEST observations of N=48+2 RR Lyrae stars in an area of 50 deg2 around the globular cluster ω Centauri.
Ref:	=2015A&A...574A..15F
by	FERNANDEZ-TRINCADO J.G. , VIVAS A.K., MATEU C.E., ZINN R., ROBIN A.C., VALENZUELA O., MORENO E., PICHARDO B.
	Astron. Astrophys., 574A, 15-15 (2015)
	Searching for tidal tails around ω Centauri using RR Lyrae stars.
o	Table 1-2: <[FVM2015] NN> (Nos 1-50).
=E=	Catalogue in electronic form as <J/A+A/574/A15/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FVR2001]
[FVR2001]	(Fruchter+Vreeswijk+Rhoads+, 2001)
Write:	<<[FVR2001] GRB 011211 abs N.NN>>
N:	1
Object:	Absorber
Note:	VLT FORS spectroscopy of GRB 011211.
Ref:	=2001GCN..1200....1F
by	FRUCHTER A. , VREESWIJK P., RHOADS J., BURUD I.
	GRB Coordinates Network, Circular Service, 1200, 1-None (2001)
	GRB 011211: optical spectroscopy.
o	<[FVR2001] GRB 011211 abs N.NN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FVW
FVW	(Forbidden-Velocity Wing)
Write:	<<FVW LLL.l+BB.b>>
N:	87+1
Object:	HI (SIMBAD class: HI = HI (21cm) Source)
Note:	Search for faint H I 21 cm emission line wings at velocities forbidden by galactic rotation in the Galactic Plane. Use of Leiden/Dwingeloo HI survey and HI Southern Galactic Plane survey data.
Ref:	=2007ApJS..173...85K
by	KANG J.-H. , KOO B.-C.
	Astrophys. J., Suppl. Ser., 173, 85-103 (2007)
	Faint H I 21 cm emission line wings at forbidden velocities.
o	Table 2: <FVW LLL.l+BB.b> N=87.
Ref:	=2012AJ....143...75K
by	KANG J.-H. , KOO B.-C., SALTER C.
	Astron. J., 143, 75 (2012)
	An old supernova remnant within an H II complex at ℓ ~ 173°: FVW 172.8+1.5.
o	<FVW LLL.l+BB.b> (No. 172.8+1.5) added.
=E=	Catalogue in electronic form as J/ApJS/173/85
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [FVW2009]
[FVW2009]	(Fang+van Boekel+Wang+, 2009)
Write:	<<[FVW2009] LNNNNA NNN>> <<[FVW2009] NN>>
N:	132+267
Object:	YSO + Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Stat:	is completely incorporated in Simbad
Note:	VLT VIMOS optical spectroscopy in the direction of the L1630N and L1641 star-forming clouds.
in source:	LDN 1641
in source:	[FM2008] NGC 2068-2071 Cluster
Ref:	=2009A&A...504..461F
by	FANG M. , VAN BOEKEL R., WANG W., CARMONA A., SICILIA-AGUILAR A., HENNING T.
	Astron. Astrophys., 504, 461-489 (2009)
	Star and protoplanetary disk properties in Orion's suburbs.
o	Tables 3-11: <[FVW2009] LNNNNA NNN> N=132+267.
=E=	Catalogue in electronic form as J/A+A/504/461
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FW2004]
[FW2004]	(Francis+Williger, 2004)
Write:	<<[FW2004] B1>> <<[FW2004] QSO J2142-4420 abs N.NNNN>>
N:	1+2
Object:	Pair of G + G in Pair (SIMBAD class: GinPair = Galaxy in Pair of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	UCLES observations on AAT. The possible member of the protocluster ClG J2142-4420 identified as [FWW2001] QSO J2142-4420 abs 2.38 is a pair of galaxies named 'B1' here, and composed of two galaxies with redshift 2.3797 and 2.3804. See also [FWW2001].
Ref:	=2004ApJ...602L..77F
by	FRANCIS P.J. , WILLIGER G.M.
	Astrophys. J., 602, 77-79 (2004)
	Low-metallicity gas clouds in a galaxy protocluster at redshift 2.38.
o	QSO J2142+4420 = QSO 2139-4434
o	<[FW2004] B1> N=1. <[FW2004] QSO J2142+4420 abs N.NNNN> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FW2006]
[FW2006]	(Fairall+Woudt, 2006)
Write:	<<[FW2006] NNNN>>
N:	295
Object:	G (SIMBAD class: Galaxy)
Note:	Spectroscopy at the 1.9m telescope at the South African Astronomical Observatory. Sample of galaxies near the SGP.
Ref:	=2006MNRAS.366..267F
by	FAIRALL A.P. , WOUDT P.A.
	Mon. Not. R. Astron. Soc., 366, 267-273 (2006)
	A sample of galaxies near the South Celestial Pole.
o	Table 1: <[FW2006] NNNN> (Nos 191, 285, 839, 1201-1490).
=E=	Catalogue in electronic form as J/MNRAS/366/267
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FW2011]
[FW2011]	(Friedel+Widicus Weaver, 2011)
Write:	<<[FW2011] JHHMMSS.sss+DDMMSS.sss>> <<[FW2011] JHHMMSS.ss+DDMMSS.ss>> <<[FW2011] CNN>>
N:	34+30+1
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	CARMA 3mm observations of the Orion-KL region.
in source:	NAME Orion KL
Ref:	=2011ApJ...742...64F
by	FRIEDEL D.N. , WIDICUS WEAVER S.L.
	Astrophys. J., 742, 64 (2011)
	A high spatial resolution study of the λ = 3 mm continuum of Orion-KL.
o	Fig. 3, Tables 1-2 col(1): <[FW2011] CNN> (Nos C1-C34) = Table 1: <[FW2011] JHHMMSS.sss+DDMMSS.sss> N=30, <[FW2011] JHHMMSS.ss+DDMMSS.ss> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FWB2009]
[FWB2009]	(Farrell+Webb+Barret+, 2009)
Write:	<<[FWB2009] HLX-1>>
N:	1
Object:	ULX (SIMBAD class: ULX = Ultra-luminous X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Use of the 2XMM Serendipitous Source catalogue to identify an ultraluminous X-ray source in ESO 243-49.
in source:	ESO 243-49
Ref:	=2009Natur.460...73F
by	FARRELL S.A. , WEBB N.A., BARRET D., GODET O., RODRIGUES J.M.
	Natur, 460, 73-75 (2009)
	An intermediate-mass black hole of over 500 solar masses in the galaxy ESO 243-49.
o	<[FWB2009] HLX-1> N=1.
Details on Acronym: [FWB89]
[FWB89]	(Faber+Wegner+Burstein+, 1989)= (Group) = (7S)
Write:	<<[FWB89] Galaxy NNN>> <<[FWB89] GrG NNN>>
N:	577+136
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	Photometric and spectroscopic data for a survey of the nearest and brightest elliptical galaxies. N=577 galaxies, and N=136 groups of galaxies.
Ref:	=1989ApJS...69..763F
by	FABER S.M. , WEGNER G., BURSTEIN D., DAVIES R.L., DRESSLER A., LYNDEN-BELL D., TERLEVICH R.J.
	Astrophys. J., Suppl. Ser., 69, 763-808 (1989)
	Spectroscopy and photometry of elliptical galaxies. VI. Sample selection and data summary.
o	Numbering 'NNN' in table 3 is not used in SIMBAD.
o	Table 1: <[FWB89] Galaxy NNN> (Nos 1-577). Table 4: <[FWB89] GrG NNN> N=136 among (Nos 21-299).
=E=	Catalogue in electronic form as VII/176
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FWC2018]
[FWC2018]	(Fesen+Weil+Cisneros+, 2018)
Write:	<<[FWC2018] NN>>
N:	12
Object:	Dust Cloud (SIMBAD class: Cloud)
Note:	N=12 dust clouds around the Cygnus Loop identified in WISE 12 and 22µm images.
Ref:	=2018MNRAS.481.1786F
by	FESEN R.A. , WEIL K.E., CISNEROS I.A., BLAIR W.P., RAYMOND J.C.
	Mon. Not. R. Astron. Soc., 481, 1786-1798 (2018)
	The Cygnus Loop's distance, properties, and environment driven morphology.
o	Fig. 8, Table 4: <[FWC2018] NN> (Nos 1-12).
o	In Chap 5 : TYC 2688-2556-1 is a misprint for TYC 2688-1556-1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FWD91]
[FWD91]	(Forbes+Ward+DePoy, 1991)
Write:	<<[FWD91] Spot A>> <<[FWD91] Radio Nucleus>>
N:	4+1
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	N=4 IR hot spots with a similar radio position, N=1 radio nucleus. See [SGE94]
in source:	NGC 253
Ref:	=1991ApJ...380L..63F
by	FORBES D.A. , WARD M.J., DEPOY D.L.
	Astrophys. J., 380, 63-66 (1991)
	Infrared hot spots in the nucleus of NGC 253.
o	+ erratum vol. 385, L31
o	Table 2A: <[FWD91] Spot A> (Nos A-D), <[FWD91] Radio Nucleus> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FWG2006]
[FWG2006]	(Foley+Watson+Gorosabel+, 2006)
Write:	<<[FWG2006] Galaxy A>>
N:	4
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spectroscopic observations of the field around GRB 980425 using DFOSC on the Danish 1.54m telescope at La Silla.
Ref:	=2006A&A...447..891F
by	FOLEY S. , WATSON D., GOROSABEL J., FYNBO J.P.U., SOLLERMAN J., McGLYNN S., McBREEN B., HJORTH J.
	Astron. Astrophys., 447, 891-895 (2006)
	The galaxies in the field of the nearby GRB 980425/SN 1998bw.
o	Fig.1, Tables 1, 2: <[FWG2006] Galaxy A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FWG2011]
[FWG2011]	(Fadely+Willman+Geha+, 2011)
Write:	<<[FWG2011] NNN>>
N:	132
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Keck DEIMOS spectroscopy and Magellan IMACS g- and r-band imaging of Segue 3.
in source:	NAME Segue 3
Ref:	=2011AJ....142...88F
by	FADELY R. , WILLMAN B., GEHA M., WALSH S., MUNOZ R.R., JERJEN H., VARGAS L.C., DA COSTA G.S.
	Astron. J., 142, 88 (2011)
	Segue 3: an old, extremely low luminosity star cluster in the Milky Way's halo.
o	Tables 1-2: <[FWG2011] NNN> (Nos 1-132).
=E=	Catalogue in electronic form as <J/AJ/142/88/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FWG96]
[FWG96]	(Ferguson+Wyse+Gallagher, 1996) (Not yet in Simbad)
Write:	<<[FWG96] A>>
N:	13
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Maps in Plates 115-116
in source:	NGC 55
Ref:	=1996AJ....112.2567F
by	FERGUSON A.M.N. , WYSE R.F.G., GALLAGHER J.S.
	Astron. J., 112, 2567-2575 (1996)
	The spectacular ionized interstellar medium of NGC 55.
o	Table 2: <[FWG96] A> (Nos A-M)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FWH2000]
[FWH2000]	(Falcke+Wilson+Henkel+, 2000)
Write:	<<[FWH2000] HHMMSS.s+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of TXS 2226-184. N=1 elongated galaxy only at 17"2 SW of the nucleus of TXS 2226-184.
Ref:	=2000ApJ...530L..13F
by	FALCKE H. , WILSON A.S., HENKEL C., BRUNTHALER A., BRAATZ J.A.
	Astrophys. J., 530, 13-16 (2000)
	Hubble Space Telescope and Very Large Array observations of the H_{2}O gigamaser galaxy TXS 2226-184.
o	<[FWH2000] HHMMSS.s+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FWJ2004]
[FWJ2004]	(Fender+Wu+Johnston+, 2004) (Not yet in Simbad)
Write:	<<[FWJ2004] Cir X-1 Core>> <<[FWJ2004] Cir X-1 Knot A>>
N:	1+2
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Note:	See also [TFK2006].
in source:	X Cir X-1
Ref:	=2004Natur.427..222F
by	FENDER R. , WU K., JOHNSTON H., TZIOUMIS T., JONKER P., SPENCER R., VAN DER KLIS M.
	Nature, 427, 222-224 (2004)
	An ultra-relativistic outflow from a neutron star accreting gas from a companion.
o	Figs 1, 2: <[FWJ2004] Cir X-1 Core> N=1, <[FWJ2004] Cir X-1 Knot A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FWKK
FWKK	(Fomalont+Windhorst+Kristian+Kellerman)
*****	Avoid the usage of FWKK, prefer 15V
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [FWS2005]
[FWS2005]	(Fox+Wakker+Savage+, 2005)
Write:	<<[FWS2005] HE 0226-4110 HVC>> <<[FWS2005] HE 0226-4110 HVC N>> <<[FWS2005] PG 0953+414 HVC>> <<[FWS2005] PG 0953+414 HVC N>>
N:	1+4+1+2
Object:	HVC (SIMBAD class: HVCld = High-velocity Cloud)
Stat:	is completely incorporated in Simbad
Note:	HST and FUSE spectroscopic observations of HVC along the sight lines toward the active galaxies HE 0226-4110 and PG 0953+414. The observations reveal multiple components for each HVC.
Ref:	=2005ApJ...630..332F
by	FOX A.J. , WAKKER B.P., SAVAGE B.D., TRIPP T.M., SEMBACH K.R., BLAND-HAWTHORN J.
	Astrophys. J., 630, 332-354 (2005)
	Multiphase high-velocity clouds toward HE 0226-4110 and PG 0953+414.
o	Table 3: <[FWS2005] HE 0226-4110 HVC>, <[FWS2005] HE 0226-4110 HVC N> (Nos 1-4). Table 4: <[FWS2005] PG 0953+414 HVC>, <[FWS2005] PG 0953+414 HVC N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FWS69]
[FWS69]	(Fitzgerald+Wison+Stegman, 1969)
Write:	<<[FWS69] R-NN>>
N:	27+34+24+19
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Cerro Tololo Observations. Stars in four photoelectric sequences in the galactic plane. See also [FM75].
Ref:	=1969PASP...81..804F
by	FITZGERALD M.P. , WILSON W., STEGMAN J.E.
	Publ. Astron. Soc. Pac., 81, 804-814 (1969)
	Four southern photoelectric sequences.
o	Table I: <[FWS69] I-NN> (Nos 1-27). Table II: <[FWS69] II-NN> (Nos 1-34). Table III: <[FWS69] III-NN> (Nos 1-24). Table IV: <[FWS69] IV-NN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FWT2010]
[FWT2010]	(Finoguenov+Watson+Tanaka+, 2010)
Write:	<<[FWT2010] SXDFNNXGG>> <<[FWT2010] DDD.dddddd+DD.dddddd>>
N:	57+6+132
Object:	X-ray Cluster of G + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	XMM-Newton observations of the Subaru-XMM Deep Field. Use of VLT and Gemini spectroscopy.
in source:	NAME SXDF
Ref:	=2010MNRAS.403.2063F
by	FINOGUENOV A. , WATSON M.G., TANAKA M., SIMPSON C., CIRASUOLO M., DUNLOP J.S., PEACOCK J.A., FARRAH D., AKIYAMA M., UEDA Y., SMOLCIC V., STEWART G., RAWLINGS S., VAN BREUKELEN C., ALMAINI O., CLEWLEY L., BONFIELD D.G., JARVIS M.J., BARR J.M., FOUCAUD S., McLURE R.J., SEKIGUCHI K., EGAMI E.
	Mon. Not. R. Astron. Soc., 403, 2063-2076 (2010)
	X-ray groups and clusters of galaxies in the Subaru-XMM deep field.
o	Fig. 1, Tables 1, 3: <[FWT2010] SXDFNNXGG> N=57+6 among (Nos 1-92). Table 2: <[FWT2010] DDD.dddddd+DD.dddddd> N=132.
=E=	Catalogue in electronic form as <J/MNRAS/403/2063/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FWV2008]
[FWV2008]	(Freire+Wolszczan+Van Den Bergh+, 2008) (Not yet in Simbad)
Write:	<<[FWV2008] Star N>>
N:	2
Object:	* (SIMBAD class: Star)
Note:	N=2 stars near the millisecond pulsar [WAK89] M 5 Psr B.
Ref:	=2008ApJ...679.1433F
by	FREIRE P.C.C. , WOLSZCZAN A., VAN DEN BERG M., HESSELS J.W.T.
	Astrophys. J., 679, 1433-1442 (2008)
	A massive neutron star in the globular cluster M5.
o	Fig.3: <[FWV2008] Star N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FWW2001]
[FWW2001]	(Francis+Wilson+Woodgate, 2001)
Write:	<<[FWW2001] QSO JHHMM+DDMM abs N.NN>>
N:	3
Object:	Absorber
Note:	S observations on AAT and complementary CTIO observations. Lyman-alpha absorption at redshift 2.38 is found in the spectra of 3 QSOs: QSO J2141-4413, QSO J2142-4420, QSO J2142-4419. These QSOs lie behind a probable galaxy protocluster (CLG J2142-4420) at redhift 2.38. See also [FW2004].
Ref:	=2001PASA...18...64F
by	FRANCIS P.J. , WILSON G.M., WOODGATE B.E.
	Publications - Astron. Soc. Australia, 18, 64-75 (2001)
	On the gas surrounding high redshift galaxy clusters.
o	Galaxy cluster = CLG J2142-4420. Tables 1, 2: possible aborption systems not in SIMBAD.
o	<[FWW2001] QSO JHHMM+DDMM abs N.NN> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FWW96]
[FWW96]	(Francis+Woodgate+Warren+, 1996)
Write:	<<[FWW96] ANNa>> <<[FWW96] AN'>>
N:	42
Object:	Poss. G (SIMBAD class: Galaxy)
Note:	Candidate Ly-alpha high redshift G, possible members of the cluster ClG J2143-4423 at z=2.38. Galaxy B1 is a pair of galaxies with 2 components B1a and B1b, and a chain of diffuse knots B1c. No. B6 in 2004ApJ...614...75F is not the same object as No. B6 in 2004ApJ...602..545P, so No. B6 in 2004ApJ...614...75F is No. B6' in SIMBAD. (Nos C1-C5): N=5 candidates foreground galaxies. Identif. charts. See also [PTF2004], [FPT2004], [CTF2006].
in source:	ClG J2143-4423
Ref:	=1996ApJ...457..490F
by	FRANCIS P.J. , WOODGATE B.E., WARREN S.J., MOLLER P., MAZZOLINI M., BUNKER A.J., LOWENTHAL J.D., WILLIAMS T.B., MINEZAKI T., KOBAYASHI Y., YOSHII Y.
	Astrophys. J., 457, 490-499 (1996)
	A group of galaxies at redshift 2.38.
o	Table 1, Fig. 3: <[FWW96] AN> (Nos B1-B3) and (Nos C1-C5)
Ref:	=1997ApJ...482L..25F
by	FRANCIS P.J. , WOODGATE B.E., DANKS A.C.
	Astrophys. J., 482, 25-28 (1997)
	A group of red, Lyα-emitting, high-redshift galaxies.
o	Table 1: <[FWW96] B4> added
Ref:	=2001ApJ...554.1001F
by	FRANCIS P.J. , WILLIGER G.M., COLLINS N.R., PALUNAS P., MALUMUTH E.M., WOODGATE B.E., TEPLITZ H.I., SMETTE A., SUTHERLAND R.S., DANKS A.C., HILL R.S., LINDLER D., KIMBLE R.A., HEAP S.R., HUTCHINGS J.B.
	Astrophys. J., 554, 1001-1011 (2001)
	A pair of compact red galaxies at redshift 2.38, immersed in a 100 kiloparsec scale Lyα nebula.
o	2142-4420 B1 = [FWW96] B1 (2000 coord.)
o	Fig.2, Table 3: <[FWW96] ANa> (Nos B1a to B1c) added.
Ref:	=2004ApJ...602..545P
by	PALUNAS P. , TEPLITZ H.I., FRANCIS P.J., WILLIGER G.M., WOODGATE B.E.
	Astrophys. J., 602, 545-554 (2004)
	The distribution of Lyα-emitting galaxies at z=2.38.
o	Table 2: <[FWW96] AN> (Nos B5-B7) added. Table 2: <[PTF2004] JHHMMSS.ss+DDMMSS.s> N=37. Table 3: <[PTF2004] JHHMMSS.ss+DDMMSS.ss> N=8.
Ref:	=2004ApJ...614...75F
by	FRANCIS P.J. , PALUNAS P., TEPLITZ H.I., WILLIGER G.M., WOODGATE B.E.
	Astrophys. J., 614, 75-83 (2004)
	The distribution of lyα-emitting galaxies at z=2.38. II. Spectroscopy.
o	Table 1: No. B6 is not the same as in 2004ApJ...602..545P, so this new object is designated as [FWW96] B6' in SIMBAD. Table 2: [FWW96] B6 (from 2004ApJ...602..545P) = [FWW96] 22 here. Table 1, Fig.7: objects b184, u093, u143, u194, P13 not identified.
o	Tables 1, 2: <[FWW96] ANN> N=22 among (Nos B10-B40), <[FWW96] AN'> (No. B6'). Tables 3, 4: <[FPT2004] JHHMMSS.ss+DDMMSS.s> N=58+43.
Ref:	=2006ApJ...637L..89C
by	COLBERT J.W. , TEPLITZ H., FRANCIS P., PALUNAS P., WILLIGER G.M., WOODGATE B.
	Astrophys. J., 637, 89-92 (2006)
	Ultraviolet-bright, high-redshift ultraluminous infrared galaxies.
o	T. 1, Fig.1 : Blob B6 is [FWW96] B6' = [PTF2004] J214242.63-443009.0 in SIMBAD.
o	Table 1: <[FWW96] BN> (Nos B8-B9) added. Table 1: <[CTF2006] JHHMMSS.ss+DDMMSS.s> N=3.
Ref:	=2013MNRAS.428...28F
by	FRANCIS P.J. , DOPITA M.A., COLBERT J.W., PALUNAS P., SCARLATA C., TEPLITZ H., WILLIGER G.M., WOODGATE B.E.
	Mon. Not. R. Astron. Soc., 428, 28-39 (2013)
	Hot gas, cold gas and sub-haloes in a Lyman α blob at redshift 2.38.
o	Text: <[FWW96] ANN> (Nos B29-B30) added.
o	LAB 1 = [SAS2000] Blob 1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FWW97]
[FWW97]	(Folgheraiter+Warwick+Watson+, 1997)
Write:	<<[FWW97] A>>
N:	3
Object:	Hotspot in SNR (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT, ASCA observations. N=3 X-ray hotspots in SNR 32.1-0.9
in source:	SNR G032.1-00.9
Ref:	=1997MNRAS.292..365F
by	FOLGHERAITER E.L. , WARWICK R.S., WATSON M.G., KOYAMA K.
	Mon. Not. R. Astron. Soc., 292, 365-377 (1997)
	G 32.1 - 0.9: a new Galactic supernova remnant?
o	Table 2: <[FWW97] A> (Nos A-C)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FWY2019]
[FWY2019]	(Fan+Wang+Yang+, 2019)
Write:	<<[FWY2019] J0439+1634 system>> <<[FWY2019] J0439+1634 lens>> <<[FWY2019] UHS J043947.08+163415.7>>
N:	1+1+1
Object:	Grav. lens system + Grav. lens + QSO (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=1 strongly lensed quasar by N=1 lensing galaxy in N=1 gravitational lensing system. Use of UKIRT Hemisphere Survey (UHS) in the near-infrared J-band, the Pan-STARRS1 survey (PS-1) at optical wavelengths, the Wide-field Infrared Survey Explorer (WISE) archive in the mid-infrared.
Ref:	=2019ApJ...870L..11F
by	FAN X. , WANG F., YANG J., KEETON C.R., YUE M., ZABLUDOFF A., BIAN F., BONAGLIA M., GEORGIEV I.Y., HENNAWI J.F., LI J., McGREER I.D., NAIDU R., PACUCCI F., RABIEN S., THOMPSON D., VENEMANS B., WALTER F., WANG R., WU X.-B.
	Astrophys. J., 870L, 11-11 (2019)
	The discovery of a gravitationally lensed quasar at z = 6.51.
o	<[FWY2019] J0439+1634 system> N=1. <[FWY2019] J0439+1634 lens> N=1. <[FWY2019] UHS J043947.08+163415.7> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: FX
FX	(Flaccomio+, X-ray) (Not yet in Simbad)
*****	Avoid the usage of FX, prefer [FMS2000]
Origin	of the Acronym: L (1999A&A...345..521F,2004AJ....127.2659R)
Details on Acronym: FXP
FXP	(Flaring X-ray Pulsar)
Write:	<<FXP HHMM+DD>>
Object:	Flaring (X) Psr (SIMBAD class: HighMassXBin = High Mass X-ray Binary)
Stat:	is completely incorporated in Simbad
Note:	FXP 0520-66 near N49 in the LMC was the first flaring X-ray pulsar observed. Its first observation was published in 1979SvAL....5..163M
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1982Ap&SS..84..173M
by	MAZETS E.P. , GOLENETSKII S.V., GURYAN Y.A., ILYINSKII V.N.
	Astrophys. Space Sci., 84, 173-189 (1982)
	The 5 March 1979 event and the distinct class of short γ bursts : are they of the same origin ?
o	<FXP 0520-66>
Details on Acronym: [FY2004]
[FY2004]	(Fang+Yao, 2004)= (NIRS) = (NIRSe)
Write:	<<[FY2004] NIRS NN>> <<[FY2004] NIRSe NN>> <<[FY2004] H2 NN>>
N:	76+30+14
Object:	(IR) + H2 (SIMBAD class: Infrared = Infra-Red Source)
Note:	NIR observations of the star formation region GGD 12-15 with the OASIS camera at the 1.88m Okayama telescope. N=76 NIRS sources, and N=30 deeply embedded NIRSe sources. N=14 H2 molecular emission knots.
in source:	NAME GGD 12-15
Ref:	=2004ChA&A..28..308F
by	FANG M. , YAO Y.-Q.
	Chinese Astron., 28, 308-322 (2004)
	Near infrared observations of the star formation region GGD 12-15.
o	Par. 3.1 : AFGL 51577 is a misprint for AFGL 5157. Par 4.4 : IC 248 is a misprint for IC 348.
o	Table 1: <[FY2004] NIRS NN> (Nos 1-76). Table 2: <[FY2004] NIRSe NN> (Nos 1-30). Table 3: <[FY2004] H2 NN> (Nos 1-14).
=E=	Catalogue in electronic form as J/other/ChA+A/28.308
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FYF2006]
[FYF2006]	(Fukui+Yamamoto+Fujishita+, 2006)
Write:	<<[FYF2006] loop N>>
N:	2+1
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	NANTEN 4m telescope CO(1-0) observations of molecular loops in the Galactic Center.
in source:	NAME Galactic Center
Ref:	=2006Sci...314..106F
by	FUKUI Y. , YAMAMOTO H., FUJISHITA M., KUDO N., TORII K., NOZAWA S., TAKAHASHI K., MATSUMOTO R., MACHIDA M., KAWAMURA A., YONEKURA Y., MIZUNO N., ONISHI T., MIZUNO A.
	Sci, 314, 106-109 (2006)
	Molecular loops in the Galactic Center: evidence for magnetic flotation.
o	<[FYF2006] loop N> (Nos 1-2).
Ref:	=2009PASJ...61.1039F
by	FUJISHITA M. , TORII K., KUDO N., KAWASE T., YAMAMOTO H., KAWAMURA A., MIZUNO N., ONISHI T., MIZUNO A., MACHIDA M., TAKAHASHI K., NOZAWA S., MATSUMOTO R., FUKUI Y.
	PASJ, 61, 1039-1053 (2009)
	Discovery of molecular loop 3 in the Galactic Center: Evidence for a positive-velocity magnetically floated loop towards L = 355°–359°.
o	Text: <[FYF2006] loop N> (No. 3) added. Table 1: <[FTK2009] MGC 355.5-0.7>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FYL2010]
[FYL2010]	(Fadda+Yan+Lagache+, 2010)
Write:	<<[FYL2010] {U\|L}NNNNN>> <<[FYL2010] SST24 JHHMMSS.ss+DDMMSS.s>>
N:	48
Object:	IR luminous G (SIMBAD class: Galaxy)
Note:	Spitzer IRS observations of N=48 infrared-luminous galaxies in the GOODS-South field (N=24 ULIRGs and N=24 LIRGs).
in source:	NAME GOODS South Field
Ref:	=2010ApJ...719..425F
by	FADDA D. , YAN L., LAGACHE G., SAJINA A., LUTZ D., WUYTS S., FRAYER D.T., MARCILLAC D., LE FLOC'H E., CAPUTI K., SPOON H.W.W., VEILLEUX S., BLAIN A., HELOU G.
	Astrophys. J., 719, 425-450 (2010)
	Ultra-deep mid-infrared spectroscopy of luminous infrared galaxies at z ~ 1 and z ~ 2.
o	Tables 2-3: <[FYL2010] ANNNNN> N=48 among (Nos U428-U16526, L3832-L16005) = <[FYL2010] SST24 JHHMMSS.ss+DDMMSS.s> N=48.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FYO2000]
[FYO2000]	(Furusho+Yamasaki+Ohashi+, 2000)
Write:	<<[FYO2000] N>>
N:	9
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ASCA observations of a region containing IRAS 20386+6751 in LDN 1157.
in source:	LDN 1157
Ref:	=2000PASJ...52..677F
by	FURUSHO T. , YAMASAKI N.Y., OHASHI T., SAITO Y., VOGES W.
	Publ. Astron. Soc. Jap., 52, 677-684 (2000)
	X-ray observation of the Lynds 1157 dark cloud region with ASCA.
o	Table 2: <[FYO2000] N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FYS2010]
[FYS2010]	(Fu+Yan+Scoville+, 2010)
Write:	<<[FYS2010] MIPS NNNNN>>
N:	52
Object:	G (SIMBAD class: Galaxy)
Note:	Spitzer IRS observations of N=52 galaxies in the COSMOS field. Use of S-COSMOS MIPS 24µm data.
in source:	NAME COSMOS Field
Ref:	=2010ApJ...722..653F
by	FU H. , YAN L., SCOVILLE N.Z., CAPAK P., AUSSEL H., LE FLOC'H E., ILBERT O., SALVATO M., KARTALTEPE J.S., FRAYER D.T., SANDERS D.B., SHETH K., TANIGUCHI Y.
	Astrophys. J., 722, 653-667 (2010)
	Decomposing star formation and active galactic nucleus with Spitzer mid-infrared spectra: luminosity functions and co-evolution.
o	Table 1: <[FYS2010] MIPS NNNNNN> N=52 among (Nos 2176-51982).
Details on Acronym: [FYS2020]
[FYS2020]	(Fukushima+Yamaguchi+Slane+, 2020)
Write:	<<[FYS2020] NN>>
N:	49
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS-I observations of N=49 point-like X-ray sources in SNR G344.7-00.1.
in source:	SNR G344.7-00.1
Ref:	=2020ApJ...897...62F
by	FUKUSHIMA K. , YAMAGUCHI H., SLANE P.O., PARK S., KATSUDA S., SANO H., LOPEZ L.A., PLUCINSKY P.P., KOBAYASHI S.B., MATSUSHITA K.
	Astrophys. J., 897, 62-62 (2020)
	Element stratification in the middle-aged SN Ia remnant G344.7-0.1.
o	Tables 2+6: <[FYS2020] NN> (Nos 1-49).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FZB2005]
[FZB2005]	(Fritz+Ziegler+Bower+, 2005)
Write:	<<[FZB2005] NNNN>>
N:	48+4
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Calar Alto 3.5m telescope spectroscopy and 5.1m Hale telescope photometry of galaxies in ACO 2390. Use of HST archival data.
in source:	ACO 2390
Ref:	=2005MNRAS.358..233F
by	FRITZ A. , ZIEGLER B.L., BOWER R.G., SMAIL I., DAVIES R.L.
	Mon. Not. R. Astron. Soc., 358, 233-255 (2005)
	On the evolutionary status of early-type galaxies in clusters at z~ 0.2 - I. The Fundamental Plane.
o	Fig.2, Tables B1, B2: <[FZB2005] NNNN> N=48+4 among (Nos 803-6666).
=E=	Catalogue in electronic form as J/MNRAS/358/233
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FZD2017]
[FZD2017]	(Figueira+Zavagno+Deharveng+, 2017)
Write:	<<[FZD2017] NNN>>
N:	122
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Herschel PACS and SPIRE photometric observations of N=122 IR sources in the bubble of the RCW 120 region. Use of archival 2MASS, Spitzer GLIMPSE and MIPSGAL data. See also [DZS2009].
in source:	RCW 120
Ref:	=2017A&A...600A..93F
by	FIGUEIRA M. , ZAVAGNO A., DEHARVENG L., RUSSEIL D., ANDERSON L.D., MEN'SHCHIKOV A., SCHNEIDER N., HILL T., MOTTE F., MEGE P., LELEU G., ROUSSEL H., BERNARD J.-P., TRAFICANTE A., PARADIS D., TIGE J., ANDRE P., BONTEMPS S., ABERGEL A.
	Astron. Astrophys., 600A, 93-93 (2017)
	Star formation towards the Galactic H II region RCW 120. Herschel observations of compact sources.
o	Table A.1: <[FZD2017] NNN> N=122 among (Nos 1-329).
=E=	Catalogue in electronic form as J/A+A/600/A93
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FZG2013]
[FZG2013]	(Fang+Zhang+Garcia-Benito+, 2013)
Write:	<<[FZG2013] PNN>>
N:	3
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Palomar 5-m Hale telescope spectroscopic observations of N=3 planetary nebulae (PNe) in the Northern Spur of M31. See also [FGG2015].
in source:	M 31 = NGC 224
Ref:	=2013ApJ...774..138F
by	FANG X. , ZHANG Y., GARCIA-BENITO R., LIU X.-W., YUAN H.-B.
	Astrophys. J., 774, 138 (2013)
	Spectroscopic observations of planetary nebulae in the northern spur of M31.
o	Table 1: <[FZG2013] PNN> (Nos PN1-PN3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FZH2010]
[FZH2010]	(Finch+Zacharias+Henry, 2010)
Write:	<<[FZH2010] UPM JHHMM+DDMM>>
N:	32
Object:	(SIMBAD class: = Double or Multiple Star)
Stat:	is completely incorporated in Simbad
Note:	N=32 common proper motion systems in the southern sky. See also UPM.
Ref:	=2010AJ....140..844F
by	FINCH C.T. , ZACHARIAS N., HENRY T.J.
	Astron. J., 140, 844-869 (2010)
	UCAC3 proper motion survey. I. Discovery of new proper motion stars in UCAC3 with 0.40"/yr > µ ≥ 0.18"/yr between declinations -90° and -47°.
o	Table 2: <UPM JHHMM+DDMMA> N=474, <[FZH2010] UPM JHHMM+DDMM> N=32.
=E=	Catalogue in electronic form as J/AJ/140/844
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FZH2011]
[FZH2011]	(Fesen+Zastrow+Hammell+, 2011) (Not yet in Simbad)
Write:	<<[FZH2011] NN>> <<[FZH2011] A>>
N:	15+8
Object:	Ejecta Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST WFPC2 and ACS observations of Cassiopeia A.
in source:	NAME Cas A
Ref:	=2011ApJ...736..109F
by	FESEN R.A. , ZASTROW J.A., HAMMELL M.C., SHULL J.M., SILVIA D.W.
	Astrophys. J., 736, 109 (2011)
	Ejecta knot flickering, mass ablation, and fragmentation in Cassiopeia A.
o	Fig. 3, Table 1: <[FZH2011] NN> (Nos 115). Fig. 5, Table 2: <[FZH2011] A> (Nos A-H).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FZM2001]
[FZM2001]	(Fabbiano+Zezas+Murray, 2001) (Not yet in Simbad)
Write:	<<[FZM2001] A>>
N:	6
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS observations of The Antennae galaxies. (Nos A-F), regions with H-alpha and X-ray emission.
in source:	NAME the Antennae
Ref:	=2001ApJ...554.1035F
by	FABBIANO G. , ZEZAS A., MURRAY S.S.
	Astrophys. J., 554, 1035-1043 (2001)
	Chandra observations of ``The Antennae'' galaxies (NGC 4038/9).
o	<[FZM2001] A> (Nos A-F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [FZM2004]
[FZM2004]	(Finn+Zaritsky+McCarthy, 2004)
Write:	<<[FZM2004] NN>>
N:	94
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	NIR observations at the 6.5m MMT of ClG J0023+0423 cluster galaxies at z about 0.8.
in source:	ClG J0023+0423
Ref:	=2004ApJ...604..141F
by	FINN R.A. , ZARITSKY D., McCARTHY D.W.Jr
	Astrophys. J., 604, 141-152 (2004)
	Hα-derived star formation rates for the z = 0.84 galaxy cluster Cl J0023+0423B.
o	Table 2: <[FZM2004] NN> (Nos 1-94).
=E=	Catalogue in electronic form as J/ApJ/604/141
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: G
G	(Gaston) (Not yet in Simbad)
*****	Avoid the usage of G, prefer BG
Origin	of the Acronym: L = Found in the literature
Details on Acronym: G
G	(Goldstone obs. source) (Not yet in Simbad)
*****	Avoid the usage of G, prefer [R75]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: G
G	(Galaxy)
*****	Avoid the usage of G, prefer [ACS96]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: G
G	(Group of G)
*****	Avoid the usage of G, prefer DV
Origin	of the Acronym: L = Found in the literature
Details on Acronym: G
G	(Member of Grand Nuage Magellan)
Note:	Liste G, member of 'Grand Nuage de Magellan',
Details on Acronym: G
G	(Giclas)= Giclas
Write:	<<G FFF-NNNA>> <<G FFF-NNNW>> <<G FFF-{B\|D}NNA>> <<G FFF{B\|D}NN A>>
N:	11923
Object:	PM* (SIMBAD class: HighPM* = High Proper Motion Star)
Note:	In the format 'B' or 'D' designate Binaries with contrasting colors. suffix A or B is added for the designation of the primary or secondary. 1971LowPM.C......0G: Recapitulation of more detailed lists published for the Northern hemisphere, in Lowell Obs. Bull. Nos 4 p.136 (1959), 5 p.61 (1961), 6 p.1 (1963), 6 p.103 (1964), 6 p.197 (1965), 6 p.233 (1966), 6 p.271 (1966), 7 p.1 (1967), 7 p.31 (1967), 7 p.67 (1968), 7 p.129 (1969), 7 p.149 (1969), 7 p.165 (1970). 1978LowOB...8...89G: Recapitulation of more detailed lists for the Southern hemisphere. Lowell Obs. Bull. 120 to 163: In Appendix, the Lowell Obs. Bull. 120, 122, 124, 132, 136, 140, 152, 158, 160, 162, 163 (ranging from 1963 to 1980) define suspected double stars with contrasting colors, with the format GFFF-BNN
Ref:	=1971LowPM.C......0G
by	GICLAS H.L. , BURNHAM R., THOMAS N.G.
	Lowell Proper Motion Survey, 0-None (1971)
	Lowell Proper Motion Survey, Northern Hemisphere. The G numbered stars.
o	<G FFF-NNNA> N=8991
Ref:	=1978LowOB...8...89G
by	GICLAS H.L. , BURNHAM R.Jr, THOMAS N.G.
	Lowell Obs. Bull., 8, 89-144 (1978)
	Lowell proper motion survey. Southern Hemisphere. Catalog 1978.
o	part no 164
o	<G FFF-NNNA> N=2758
=E=	Catalogue in electronic form as I/79
=E=	Catalogue in electronic form as I/112
Details on Acronym: G
G	(Gavazzi)
Origin	of the Acronym: L (1993ApJS...85....1N)
Details on Acronym: G
G	(Goodman+Bastien+Myers+, 1990)
*****	Avoid the usage of G, prefer [GBM90]
Origin	of the Acronym: L (1997ApJ...491L.103A)
Details on Acronym: G
G	(Garnavich+)
*****	Avoid the usage of G, prefer [GNG92]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: G
G	(Galactic)
Rem:	Systematic designation
*****	Avoid the usage of G, prefer GRS
Details on Acronym: G
G	(Gum)
*****	Avoid the usage of G, prefer Gum
Details on Acronym: G
G	(Grande vitesse)
*****	Avoid the usage of G, prefer GV
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: G
G	(cloud complex labelled G)
*****	Avoid the usage of G, prefer [H68]
Details on Acronym: G
G	(Giclas)
*****	Avoid the usage of G, prefer HG
Details on Acronym: G
G	(Globular Cl)
*****	Avoid the usage of G, prefer [HGH92]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: G
G	(Galaxy)
*****	Avoid the usage of G, prefer JJ
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: G
G	(Galaxy)
*****	Avoid the usage of G, prefer [KTF96]
Origin	of the Acronym: L (2004ApJS..150...43G)
Details on Acronym: G
G	(Galactic PN)
*****	Avoid the usage of G, prefer PN
Origin	of the Acronym: L = Found in the literature
Details on Acronym: G
G	(Greenwich)
*****	Avoid the usage of G, prefer RGO
Origin	of the Acronym: L = Found in the literature
Details on Acronym: G
G	(GCl)
*****	Avoid the usage of G, prefer SKHB
Origin	of the Acronym: L = Found in the literature
Details on Acronym: G
G	(Giant)
*****	Avoid the usage of G, prefer WOH
Origin	of the Acronym: L = Found in the literature
Details on Acronym: G
G	(Galaxy)
*****	Avoid the usage of G, prefer YGKOW
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: G		G
G	G	(Georgelin+Georgelin)
*****	Avoid the usage of G	G, prefer [GG76]
Origin	of the Acronym: L (1997ApJ...476..347Y)
Details on Acronym: G-G
G-G	(Gonzalez+Gonzalez) (Not yet in Simbad)
*****	Avoid the usage of G-G, prefer GGE
Origin	of the Acronym: L = Found in the literature
Details on Acronym: G-G
G-G	(Gonzalez+Gonzalez)
*****	Avoid the usage of G-G, prefer GGA
Origin	of the Acronym: L = Found in the literature
Details on Acronym: G-G
G-G	(Gonzalez+Gonzalez)
*****	Avoid the usage of G-G, prefer GGR
Origin	of the Acronym: L = Found in the literature
Details on Acronym: G-G
G-G	(Gonzalez+Gonzalez)
*****	Avoid the usage of G-G, prefer [GG52]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: G-G
G-G	(Gonzalez+Gonzalez)
*****	Avoid the usage of G-G, prefer [GG53]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: G-Gamma
G-Gamma	(Gal. gamma-ray)= (Gamma) (Not yet in Simbad)
Write:	<<G-Gamma LLL+BB>>
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Rem:	Obsolete
Details on Acronym: G.R.
G.R.	(G. Reaves)
*****	Avoid the usage of G.R., prefer GRDG
Details on Acronym: 1G
1G	(Gonzalez+, 1st list)
*****	Avoid the usage of 1G, prefer GGA
Origin	of the Acronym: L (1970MmRAS..73..153W)
Details on Acronym: 2G
2G	(Gonzalez+, 2nd list) (Not yet in Simbad)
*****	Avoid the usage of 2G, prefer GGE
Origin	of the Acronym: L (1970MmRAS..73..153W)
Details on Acronym: [G2000]
[G2000]	(Gallimore, 2000)
Write:	<<[G2000] JHHMMSS.ssss+DDMMSS.sss>>
N:	1
Object:	Poss. SNR (SIMBAD class: SNRemnant_Candidate = SuperNova Remnant Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=1 SNR candidate in the field of NGC 6240. See also [CTH90] and [BRS93].
Ref:	=2000IAUC.7428Q...1G
by	GALLIMORE J.F.
	IAU Circ., 7428, 1-None (2000)
	Possible radio supernova in NGC 6240.
o	galaxy nuclei are [BRS93] B (North) and A (South).
o	<[G2000] JHHMMSS.ssss+DDMMSS.sss> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G2001]
[G2001]	(Green, 2001)= ([G2001a])
Write:	<<[G2001] G353.9-2.0 W>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=2 radio VLA components of SNR 353.9-2.0.
in source:	SNR G353.9-02.0
Ref:	=2001MNRAS.326..283G
by	GREEN D.A.
	Mon. Not. R. Astron. Soc., 326, 283-286 (2001)
	G353.9-2.0, a new Galactic supernova remnant identified from the NRAO Very Large Array Sky Survey.
o	Table 2: <[G2001a] G353.9-2.0 W> (Nos E, W).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G2001a]
[G2001a]	(Green, 2001)
*****	Avoid the usage of [G2001a], prefer [G2001]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G2001b]
[G2001b]	(Goranskii, 2001)
Write:	<<[G2001b] N>> <<[G2001b] a>>
N:	6+2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=6 primary standard stars (Nos 1-6), N=1 comparison star (No. c), N=1 check star (No. k), in the field of BQ Cam.
Ref:	=2001AstL...27..516G
by	GORANSKII V.P.
	Astron. Lett., 27, 516-520 (2001)
	Photometric study of BQ Camelopardalis, an optical counterpart of the X-ray source V0332+53.
o	Table 2: <[G2001b] N> (Nos 1-6), <[G2001b] a> (Nos c, k).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G2004]
[G2004]	(Greaves, 2004)
Write:	<<[G2004] NNN>> <<[G2004] NNNAA>>
N:	972+1947
Object:	** + i* (SIMBAD class: ** = Double or Multiple Star)
Stat:	is completely incorporated in Simbad
Note:	New Northern celestial hemisphere proper-motion pairs are derived from the Second US Naval Observatory CCD Astrograph Catalog (see UCAC2).
Ref:	=2004MNRAS.355..585G
by	GREAVES J.
	Mon. Not. R. Astron. Soc., 355, 585-590 (2004)
	New Northern hemisphere common proper-motion pairs.
o	Table 1: <[G2004] NNN> (Nos 1-972). Table 1: <[G2004] NNNA> N=969x2+3x3.
=E=	Catalogue in electronic form as J/MNRAS/355/585
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G2005]
[G2005]	(Gondoin, 2005)
Write:	<<[G2005] NN>>
N:	58
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of the stellar cluster NGC 188.
in source:	NGC 188
Ref:	=2005A&A...438..291G
by	GONDOIN P.
	Astron. Astrophys., 438, 291-300 (2005)
	X-ray observations of the old open stellar cluster NGC 188.
o	in ref list Binnendijk 1970VA.....12..217B instead of VA.12.211 , KALUZNY 1987ApJ...314..585K instead of AJ.314
o	Table 1: <[G2005] NN> (Nos 1-58).
=E=	Catalogue in electronic form as J/A+A/438/291
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G2006]
[G2006]	(Gondoin, 2006)
Write:	<<[G2006] NNN>>
N:	102
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of the core of the Lupus 3 region.
in source:	Lupus 3
Ref:	=2006A&A...454..595G
by	GONDOIN P.
	Astron. Astrophys., 454, 595-607 (2006)
	X-ray emission from T Tauri stars in the Lupus 3 star-forming region.
o	Paragraph 3.1. Bianco 1 is a probable misprint for Blanco 1.
o	Table 6: <[G2006] NNN> (Nos 1-102).
=E=	Catalogue in electronic form as J/A+A/454/595
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G2011]
[G2011]	(Gyulbudaghian, 2011)
Write:	<<[G2011] cnN>> <<[G2011] cn2 IR cluster>>
N:	2+1
Object:	Compact Nebula + Cluster of * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=2 compact nebulae and N=1 associated IR star cluster in Sh 2-235. Use of archival 2MASS data.
in source:	SH 2-235
Ref:	=2011Ap.....54..384G
by	GYULBUDAGHIAN A.L.
	Ap, 54, 384-391 (2011)
	The compact nebulae CN1 and CN2, coupled to infrared stellar clusters.
o	Fig. 2, Tables 2-3: <[G2011] cnN> (Nos cn1-cn2). Table 3: <[G2011] cn2 IR cluster> N=1.
o	A translation of Astrofizika Vol. 54, No 3, pp. 433-441, 2011
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G2012]
[G2012]	(GOUDFROOIJ, 2012)= ([G2012a])
Write:	<<[G2012] NNN>>
N:	478 (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST ACS observations of NGC 1316.
in source:	NGC 1316
Ref:	=2012ApJ...750..140G
by	GOUDFROOIJ P.
	Astrophys. J., 750, 140 (2012)
	Sizes, half-mass densities, and mass functions of star clusters in the merger remnant NGC 1316: clues to the fate of second-generation globular clusters.
o	Table 1: <[G2012] NNN> (Nos 1-478).
=E=	Catalogue in electronic form as <J/ApJ/750/140/>
Details on Acronym: [G2012a]
[G2012a]	(GOUDFROOIJ, 2012)
*****	Avoid the usage of [G2012a], prefer [G2012]
Details on Acronym: [G2012b]
[G2012b]	(Galleti, 2012)
Write:	<<[G2012b] CNNN>>
N:	45
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	List of objects discovered by Caldwell et al. 2009AJ....137...94C, but misidentified in the original paper. For more information, visit the Revised Bologna Catalog website (http://www.bo.astro.it/M31/), and see their file http://www.bo.astro.it/M31/RBC_Caldwell.txt
in source:	M 31 = NGC 224
Ref:	=2014yCat.5143....0G
by	GALLETI S. , FEDERICI L., BELLAZZINI M., FUSI PECCI F., MACRINA S., BUZZONI A.
	yCat, 5143, 0 (2014)
	Revised Bologna Catalog of M31 clusters, V.5 (Galleti+ 2012).
o	<RBC NNNNN> N=2060 among (Nos 1-10046). <[G2012b] CNNN> (Nos C002-C042).
=E=	Catalogue in electronic form as V/143
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G2014]
[G2014]	(Glushak, 2014) (Not yet in Simbad)
Write:	<<[G2014] ANN>> <<[G2014] RN'>> <<[G2014] Spot 4>>
N:	18+4+1
Object:	(X) + (Rad) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Use of VLA and Chandra data to analyze the radio and X-ray fine structure of SNR G011.2-00.3.
in source:	SNR G011.2-00.3
Ref:	=2014ARep...58....6G
by	GLUSHAK A.P.
	ARep, 58, 6-15 (2014)
	Microquasar jets in the supernova remnant G11.2-0.3.
o	Figs 1+5, Table: <[G2014] AN> (Nos X1-X9, R1-R9), <[G2014] RN'> (Nos R3'-R4', R6'-R7'), <[G2014] Spot 4> N=1.
o	2014AZh....91....9G
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G2016]
[G2016]	(Grosbol, 2016)= (OPS) (Not yet in Simbad)
Write:	<<[G2016] OPS JHHMMSSs+DDMMSS>>
N:	12675
Object:	Early-type * (SIMBAD class: Star)
Note:	N=12675 early-type stars towards the Galactic center. Use of objective prism plates obtained with the 4° prism on the ESO 1m Schmidt telescope (La Silla) suing IIaO, 4415, and IIIaJ emulsions.
in source:	NAME Gal Center
Ref:	=2016A&A...585A.141G
by	GROSBOL P.
	Astron. Astrophys., 585A, 141-141 (2016)
	A catalog of early-type stars toward the Galactic Center.
o	<[G2016] OPS JHHMMSSs+DDMMSS> N=12675.
=E=	Catalogue in electronic form as <J/A+A/585/A141/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 3G
3G	(Gonzalez+, 3rd list)
*****	Avoid the usage of 3G, prefer GGR
Origin	of the Acronym: L (1970MmRAS..73..153W)
Details on Acronym: G3CC
G3CC	(GLIMPSE 3-Color Cluster)
Write:	<<G3CC NN>>
N:	75
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	N=75 stellar clusters detected by visual inspection of three-color images. Use of a stellar density map of the GLIMPSE point source catalog filtered by a red color criterion.
Ref:	=2013A&A...560A..76M
by	MORALES E.F.E. , WYROWSKI F., SCHULLER F., MENTEN K.M.
	Astron. Astrophys., 560A, 76-76 (2013)
	Stellar clusters in the inner Galaxy and their correlation with cold dust emission.
o	Table 2: <G3CC NN> N=69 among (Nos 5-73).
=E=	Catalogue in electronic form as J/A+A/560/A76
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: G4Jy
G4Jy	(A source belonging to the GLEAM 4-Jy (G4Jy) Sample)
Write:	<<G4Jy NNNNA>>
N:	1863+175 (SIMBAD class: Radio = Radio Source)
Note:	The GLEAM 4-Jy (G4Jy) Sample is a compilation of the brightest extragalactic radio-sources across the southern sky (Dec. < 30 deg), which have an integrated flux-density > 4 Jy at 151 MHz. Please see the following repository for further details and links: https://github.com/svw26/G4Jy
Notes:	Not all of the G4Jy sources have an identification in AllWISE yet (J2000), in which case the centroid position should be used for cross-matching with other catalogues. Furthermore, an individual component of a G4Jy source that is multi-component in GLEAM (https://arxiv.org/abs/1610.08318) has a designation of the format 'G4Jy NNNNA'.
Ref:	=arXiv:1810.01226
Ref:	=2020PASA...37...18W
by	WHITE S.V. , FRANZEN T.M.O., RISELEY C.J., WONG O.I., KAPINSKA A.D., HURLEY-WALKER N., CALLINGHAM J.R., THORAT K., WU C., HANCOCK P., HUNSTEAD R.W., SEYMOUR N., SWAN J., WAYTH R., MORGAN J., CHHETRI R., JACKSON C., WESTON S., BELL M., FOR B.-Q., GAENSLER B.M., JOHNSTON-HOLLITT M., OFFRINGA A., STAVELEY-SMITH L.
	PASA, 37, 18-18 (2020)
	The GLEAM 4-Jy (G4Jy) Sample: II. Host-galaxy identification for individual sources.
Ref:	=2020PASA...37...17W
by	WHITE S.V. , FRANZEN T.M.O., RISELEY C.J., WONG O.I., KAPINSKA A.D., HURLEY-WALKER N., CALLINGHAM J.R., THORAT K., WU C., HANCOCK P., HUNSTEAD R.W., SEYMOUR N., SWAN J., WAYTH R., MORGAN J., CHHETRI R., JACKSON C., WESTON S., BELL M., FOR B.-Q., GAENSLER B.M., JOHNSTON-HOLLITT M., OFFRINGA A., STAVELEY-SMITH L.
	PASA, 37, 17-17 (2020)
	The GLEAM 4-Jy (G4Jy) Sample: I. Definition and the catalogue.
o	<G4Jy NNNN> N=1863, <G4Jy NNNNA> N=175. Rhodes University
=E=	Catalogue in electronic form as <VIII/105/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [G55]
[G55]	(Gaposhkin, 1955)
Write:	<<[G55] NNN>>
N:	285
Object:	V* (SIMBAD class: Variable* = Variable Star)
Ref:	=1955PZ.....10..337G
by	GAPOSCHKIN S.I.
	Perem. Zvezdy, 10, 337-381 (1955)
	285 variable stars in direction of the Galactic Center.
o	Table 1, col(1): <[G55] NNN> (Nos 1-285).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G63]
[G63]	(Griffin, 1963)
Write:	<<[G63] 3C NNN a>> <<[G63] 3C NNN N>> <<[G63] M 84 a>> <<[G63] Coma A a>> <<[G63] NGC 5128 a>> <<[G63] M 23-1 a>> <<[G63] M 23-1 N>>
N:	346
Object:	* (SIMBAD class: Star)
Note:	N=346 stars in 42 fields Identif. charts in Fig.1
Ref:	=1963AJ.....68..421G
by	GRIFFIN R.F.
	Astron. J., 68, 421-428 (1963)
	Positions of optical objects in the fields of 42 radio sources.
o	Table II: <[G63] 3C NNN a>, <[G63] 3C NNN N>, <[G63] M 84 a>, <[G63] Coma A a>, <[G63] NGC 5128 a>, <[G63] M 23-1 a>, <[G63] M 23-1 N>, N=346
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G70]
[G70]	(Graham, 1970)
Write:	<<[G70] Np>> <<[G70] Sf>>
N:	1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	5GHz observations with the Cambridge One-Mile Telescope of the rG M 87.
in source:	M 87 = Virgo A = NGC 4486
Ref:	=1970MNRAS.149..319G
by	GRAHAM I.
	Mon. Not. R. Astron. Soc., 149, 319-339 (1970)
	Observations of M 87 at 5 GHz.
o	Table I: <[G70] Wa> (Nos Np, Sf).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G71]
[G71]	(Grueff, 1971)
Write:	<<[G71] HHMM+DD>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table I: Among the 224 radio-sources, two are not in the B2 catalog: 0719+32 and 1039+33.
Ref:	=1971AJ.....76..530G
by	GRUEFF G.
	Astron. J., 76, 530-536 (1971)
	Flux density measurements of optically identified B2 radio sources at 5 GHz.
o	Table I: Among the 224 sources, two are not in the B2 catalog and are designated as '[G71] 0719+32' and '[G71] 1039+33' in SIMBAD.
o	Table I: <[G71] HHMM+DD> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G74]
[G74]	(Gillespie, 1974)= (ARG) (Not yet in Simbad)
Write:	<<[G74] a>>
N:	8
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1974MNRAS.166p..11G
by	GILLESPIE A.R.
	Mon. Not. R. Astron. Soc., 166, part no 16, 11-15 (1974)
	Initial results from a radio continuum survey of the area around NGC 7331 and Stephan's Quintet.
o	Table I: <[G74] a> (Nos a-h)
Details on Acronym: [G77]
[G77]	(Graham, 1977) (Not yet in Simbad)
Write:	<<[G77] NN>>
N:	76
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	RR Lyr in the field of NGC 1783 in the LMC.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1977PASP...89..425G
by	GRAHAM J.A.
	Publ. Astron. Soc. Pac., 89, 425-465 (1977)
	The RR Lyrae stars in the Large Magellanic Cloud.
o	Table 1: <[G77] NN> (Nos 1-76).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G79]
[G79]	(Graham, 1979)
Write:	<<[G79] NN>> <<[G79] Knot X>>
N:	18+1
Object:	HII + Knot (SIMBAD class: HIIReg = HII Region)
in source:	Cen A = NGC 5128
Ref:	=1979ApJ...232...60G
by	GRAHAM J.A.
	Astrophys. J., 232, 60-73 (1979)
	The structure and evolution of NGC 5128.
o	Fig.2, Table 2: <[G79] NN> (Nos 1-18), <[G79] Knot X> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G81]
[G81]	(Graham, 1981)= ([G81a]) = (Grah)
Write:	<<[G81] NN>>
N:	17
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Stars near NGC 300
in source:	NGC 300
Ref:	=1981PASP...93...29G
by	GRAHAM J.A.
	Publ. Astron. Soc. Pac., 93, 29-31 (1981)
	A photoelectric UBVRI sequence near NGC 300 for the calibration of faint stellar magnitudes.
o	<[G81] NN> N=17
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G81a]
[G81a]	(Graham, 1981)
*****	Avoid the usage of [G81a], prefer [G81]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G81b]
[G81b]	(Graham, 1981)
Write:	<<[G81b] NN>>
N:	17
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	Cen A = NGC 5128
Ref:	=1981PASP...93..291G
by	GRAHAM J.A.
	Publ. Astron. Soc. Pac., 93, 291-293 (1981)
	Photoelectric UBVRI photometry in two fields near NGC 5128.
o	Table II: [R69] NN
o	Table I: <[G81b] NN> (Nos 1-10).
Ref:	=1982PASP...94..828M
by	McELROY D.B. , HUMPHREYS R.M.
	Publ. Astron. Soc. Pac., 94, 828-None (1982)
	UBVRI photoelectric sequences for M83 and NGC 5128.
o	Table I: <[MH82] M 83 NN> (Nos 1-14). Table II: <[G81b] NN> (Nos 11-17) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G82a]
[G82a]	(Gyulbudaghian)= (Gy)
Write:	<<[G82a] NN>>
N:	13
Object:	RFN (SIMBAD class: RefNeb = Reflection Nebula)
Stat:	is completely incorporated in Simbad
Ref:	=1982PAZh....8..222G
by	GYUL'BUDAGYAN A.L.
	Pis'ma Astron. Zh., 8, 222-223 (1982)
	New cometary nebulae.
o	Table I: <[G82a] NN> (Nos 1-13)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G82b]
[G82b]	(Gyulbudaghian, 1982)= (Gy)
Write:	<<[G82b] NN>>
N:	21
Object:	HH-like (SIMBAD class: HerbigHaroObj = Herbig-Haro Object)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-21) In ref. 1983RMxAA...8..147T ([TRC83]), the numbering is (Nos 1-22), and objects have been renumbered after a new No. 5.
Ref:	=1982PAZh....8..232G
by	GYULBUDAGHIAN A.L.
	Pis'ma Astron. Zh., 8, 232-233 (1982)
	New objects resembling Herbig-Haro ones.
o	<[G82b] NN> (Nos 1-21)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G82c]
[G82c]	(Gyulbudaghian, 1982)
Write:	<<[G82c] N>>
N:	6
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Ref:	=1982ATsir1224....7G
by	GYULBUDAGHIAN A.L.
	Astron. Tsirk., 1224, 7-8 (1982)
	Objects found during the survey of PSS.
o	<[G82c] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G83]
[G83]	(Gyulbudaghian, 1983)
Write:	<<[G83] HHMMSS+DDMM>>
N:	37
Object:	* (SIMBAD class: Star)
Note:	N=37 stars in Trapezium-like systems.
Ref:	=1983Afz....19..747G
by	GYULBUDAGHIAN A.L.
	Astrofizika, 19, 747-752 (1983)
	Trapezium like large systems.
o	Table 1: <[G83] HHMMSS+DDMM> N=37.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G84]
[G84]	(Graham, 1984)= ([G84a])
Write:	<<[G84] NN>>
N:	34
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Stat:	is completely incorporated in Simbad
in source:	NGC 300
Ref:	=1984AJ.....89.1332G
by	GRAHAM J.A.
	Astron. J., 89, 1332-1342 (1984)
	The Cepheid variables in NGC 300.
o	<[G84] NN> N=34
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G84a]
[G84a]	(Graham, 1984)
*****	Avoid the usage of [G84a], prefer [G84]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G84b]
[G84b]	(Gyulbudaghian, 1984)= (Gy)
Write:	<<[G84b] NN>>
N:	12
Object:	HH-like (SIMBAD class: HerbigHaroObj = Herbig-Haro Object)
Stat:	is completely incorporated in Simbad
Ref:	=1984Afz....20..631G
by	GYULBUDAGHIAN A.L.
	Astrofizika, 20, 631-634 (1984)
	On the objects looking like Herbig-Haro objects.
o	<[G84b] NN> (Nos 1-12)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G84c]
[G84c]	(Gyulbudaghian, 1984)= (Gy)
Write:	<<[G84c] N>>
N:	5
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1984ATsir1342....7G
by	GYULBUDAGHIAN A.L.
	Astron. Tsirk., 1342, 7-8 (1984)
	New objects found during survey PSS.
o	<[G84c] N> (Nos 1-5)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G84d]
[G84d]	(Gyulbudaghian, 1984)
Write:	<<[G84d] N-N>>
N:	8+4
Object:	Nebula + * (SIMBAD class: ISM = Interstellar Medium Object)
Stat:	is completely incorporated in Simbad
Note:	Table 1: format '1-N', N=8 cometary nebulae. Table 2: format '2-N', N=4 Trapezium-like systems.
Ref:	=1984Afz....21..185G
by	GYULBUDAGHIAN A.L.
	Astrofizika, 21, 185-188 (1984)
	New cometary nebulae and tight Trapezium-like systems.
o	Table 1: <[G84d] 1-N> (Nos 1-1 to 1-8). Table 2: <[G84d] 2-N> (Nos 2-1 to 2-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G85]
[G85]	(Gyulbudaghian, 1985)= (GRS) = ([G85a])
Write:	<<[G85] NN>>
N:	32
Object:	Dark Globule (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
in source:	NAME ASS CEP OB 2-
Ref:	=1985Afz....23..295G
by	GYULBUDAGHIAN A.L.
	Astrofizika, 23, 295-306 (1985)
	On the radial systems of dark globules.
o	<[G85] NN> (Nos 1-32)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G85a]
[G85a]	(Gyulbudaghian, 1985)= (GRS)
*****	Avoid the usage of [G85a], prefer [G85]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G85b]
[G85b]	(Graham, 1985)
Write:	<<[G85b] NN>>
N:	12
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Yale 1m telescope observations of variable stars in the LMC cluster NGC 1786.
in source:	NGC 1786
Ref:	=1985PASP...97..676G
by	GRAHAM J.A.
	Publ. Astron. Soc. Pac., 97, 676-680 (1985)
	Variable stars in the Large Magellanic Cloud cluster NGC 1786.
o	Fig. 1, Table I: <[G85b] NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G87]
[G87]	(Gavazzi, 1987)= (G)
Write:	<<[G87] NN>>
N:	19
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
in source:	NAME Coma Supercluster
Ref:	=1987ApJ...320...96G
by	GAVAZZI G.
	Astrophys. J., 320, 96-121 (1987)
	21 centimeter study of spiral galaxies in the Coma supercluster.
o	Table 2: <[G87] NN> (Nos 1-19)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G90]
[G90]	(Giraud, 1990)
Write:	<<[G90] A>> <<[G90] a>> <<[G90] NN>>
N:	11+2+56
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	ClG 0500-24
Ref:	=1990A&AS...83....1G
by	GIRAUD E.
	Astron. Astrophys., Suppl. Ser., 83, 1-10 (1990)
	Galaxy population in the cluster Cl 0500-24.
o	<[G90] A> N=11, <[G90] a> N=2, <[G90] NN> N=56
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: G91
G91	(Gallagher+, 1991)
*****	Avoid the usage of G91, prefer [GHG91]
Origin	of the Acronym: L (2006ApJ...652.1170C)
Details on Acronym: [G92]
[G92]	(Grillmair, 1992) (Not yet in Simbad)
Write:	<<[G92] NNN>>
N:	16
Object:	Cluster of * + * + G (SIMBAD class: GlobCluster = Globular Cluster)
Note:	From Grillmair Ph.D. Thesis, 1992. Selection of globular cluster candidates from a Grillmair list. N=10 globular clusters, 2 stars, and 4 galaxies. See also [KGM99].
in source:	NGC 1399
Ref:	=2001ApJ...563L.143F
by	FORBES D.A. , BEASLEY M.A., BRODIE J.P., KISSLER-PATIG M.
	Astrophys. J., 563, 143-146 (2001)
	Age estimates for globular clusters in NGC 1399.
o	Table 1: Objects from a list in Grillmair Thesis, 1992.
o	Table 1, text: <[G92] NNN> N=10+2+4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G93]
[G93]	(Grindlay, 1993)= ([G93a])
Write:	<<[G93] NGC 6397 AN>> <<[G93] NGC 6752 A>>
N:	5+4
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT sources in NGC 6397 and NGC 6752. In NGC 6397, same numbering as in CGKB.
in source:	NGC 6397
in source:	NGC 6752
Ref:	=1993ASPC...50..285G
by	GRINDLAY J.E.
	ASP Conf. Ser. 50, Proc. of a workshop held in Berkeley, California, July 15th to 17th, 1992, to hono the 65th birthday of Ivan King. "Structure and Dynamics of Globular Clusters". Ed. by S.G. Djorgovski and G. Meylan., 50, 285-295 (1993)
	Early studies of globular clusters with ROSAT.
o	Table I, Fig.1: <[G93] NGC 6397 AN> (Nos A, B, C1-C3). Table I, Fig.2: <[G93] NGC 6752 A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G93a]
[G93a]	(Grindlay, 1993)
*****	Avoid the usage of [G93a], prefer [G93]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G93b]
[G93b]	(Goodrich, 1993)
Write:	<<[G93b] Elia 3-1 Anon>> <<[G93b] HK Ori HH>> <<[G93b] HK Ori Anon>> <<[G93b] AS 310 WW>> <<[G93b] BD +41 3731 HH>> <<[G93b] BD +46 3471 HHN>>
N:	9
Object:	HH + * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Search for faint stars or new HH objects near 6 Herbig Ae/Be stars.
Ref:	=1993ApJS...86..499G
by	GOODRICH R.W.
	Astrophys. J., Suppl. Ser., 86, 499-515 (1993)
	A search for Herbig-Haro objects near Herbig Ae/Be stars.
o	(Erratum) 1993 ApJ 88, p. 609
o	Table 2: <[G93b] Elia 3-1 Anon> N=1, <[G93b] HK Ori HH> N=1, <[G93b] HK Ori Anon> N=1, <[G93b] AS 310 WWW> (Nos NE, SW), <[G93b] BD +41 3731 HH> N=1, <[G93b] BD +46 3471 HHN> (Nos HH1 to HH3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G93c]
[G93c]	(Garcia, 1993)
Write:	<<[G93c] NNN>>
N:	478
Object:	* (SIMBAD class: Star)
Note:	CTIO 1m telescope spectroscopic and Lowell 61cm and 91cm telescopes photometric observations of N=478 stars in the field of the Carina OB2 association.
in source:	Ass Car OB 2
Ref:	=1993ApJS...87..197G
by	GARCIA B.
	Astrophys. J., Suppl. Ser., 87, 197-216 (1993)
	A study of Carina OB2 association. I. Observational data.
o	Table 1: <[G93c] NNN> (Nos 1-478).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: G94
G94	(Graham+, 1994)
*****	Avoid the usage of G94, prefer [GMS94]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [G94]
[G94]	(Gwinn, 1994)
Write:	<<[G94] NNN>>
N:	271
Object:	H2O Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
in source:	W 49:W 49N = W 49N
Ref:	=1994ApJ...429..253G
by	GWINN C.R.
	Astrophys. J., 429, 253-267 (1994)
	Physical structure of H2O masers in W 49N.
o	<[G94] NNN> N=271
=E=	Catalogue in electronic form as J/ApJ/429/253
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G96]
[G96]	(Gorjian, 1996)= ([G96a]) = (V)
Write:	<<[G96] N>>
N:	6
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations. Table 1: N=6 clusters of stars in NGC 5253, Map in Fig. 2
in source:	NGC 5253
Ref:	=1996AJ....112.1886G
by	GORJIAN V.
	Astron. J., 112, 1886-1893 (1996)
	WFPC2 imaging of the starburst galaxy NGC 5253.
o	Table 1: <[G96] N> (Nos 1-6)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G96a]
[G96a]	(Gorjian, 1996)
*****	Avoid the usage of [G96a], prefer [G96]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G96b]
[G96b]	(Georgiev, 1996) (Not yet in Simbad)
Write:	<<[G96b] UGC NNNN NNN>>
N:	647+74
Object:	* (SIMBAD class: Star)
in source:	UGC 288
in source:	UGC 2905
in source:	UGC 3755
in source:	UGC 3860 = DDO 43
in source:	UGC 3966
in source:	UGC 3974
in source:	UGC 4115
in source:	UGC 5721
in source:	UGC 6541
in source:	UGC 6565
in source:	UGC 6572
in source:	UGC 6817
in source:	UGC 7559
Ref:	=1996BSAO...41...88G
by	GEORGIEV T.B.
	Bull. Special Astrophys. Obs., 41, 88-122 (1996)
	CCD stellar photometry in 13 dwarf irregular galaxies.
o	Appendix 2: <[G96b] UGC NNNN NNN> N=721
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G97]
[G97]	(Gaidos, 1997)
Write:	<<[G97] ACO NNNN BCG>>
N:	20
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=20 Brightest Cluster Galaxies (BCG) in 20 ACO
Ref:	=1997AJ....114..474G
by	GAIDOS E.J.
	Astron. J., 114, 474-481 (1997)
	Photometry of brightest galaxies in twenty Abell clusters.
o	Table 1: <[G97] ACO NNNN BCG> N=20
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: G98
G98	(Gordon+, 1998)
*****	Avoid the usage of G98, prefer M33SNR
Origin	of the Acronym: L (2005AJ....130..539G)
Details on Acronym: [G98]
[G98]	(Gyulbudaghian, 1998)= (CLN)
Write:	<<[G98] NNN>>
N:	189
Object:	Nebula (SIMBAD class: ISM = Interstellar Medium Object)
Note:	Table 1: (Nos 1-189), Cometary-like nebulae.
Ref:	=1998Ap.....41..382G
by	GYULBUDAGHIAN A.L.
	Astrophysics, 41, 382-391 (1998)
	Nonsteady objects associated with star-forming regions. Relationship to stellar associations, infrared sources, and water masers.
o	Cross-id.: G1-NN = [G82a] in table 1, [G82b] in table 2. G2-NN = [G82c] in table 1, [G84b] in table 2. G3-NN = [G84d] 1-N in table 1, [G84c] in table 2. Both designations 'G4' have not been identified (ref. not found). GM 1-NN = GM 1-NN but GM 2-NN = GM 3-NN in SIMBAD.
o	Table 1: <[G98] NNN> (Nos 1-189). Table 2: <HHL NNa> N=11.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G99]
[G99]	(Gibb, 1999)= ([G99a])
Write:	<<[G99] LBS NN cmN>>
N:	12
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=12 3.5cm sources in 5 MCld cores.
in source:	LBS 2-13
in source:	LBS 2-16
in source:	LBS 2-17
in source:	LBS 2-18
in source:	LBS 2-23
Ref:	=1999MNRAS.304....1G
by	GIBB A.G.
	Mon. Not. R. Astron. Soc., 304, 1-7 (1999)
	A VLA search for embedded young stellar objects and protostellar candidates in L1630.
o	LBS NN = LBS 2-NN in SIMBAD.
o	Table 2: <[G99] LBS NN cmN> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G99a]
[G99a]	(Gibb, 1999)
*****	Avoid the usage of [G99a], prefer [G99]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [G99b]
[G99b]	(Golla, 1999)
Write:	<<[G99b] SS.s+SSs>>
N:	20
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Format: offset relative to RA: 12h 39', Dec: +32deg 49' If Dec < 600 offset +32deg 50' (ex. Dec 653 corresponds to +32deg 50' 5.3").
in source:	NGC 4631
Ref:	=1999A&A...345..778G
by	GOLLA G.
	Astron. Astrophys., 345, 778-786 (1999)
	High resolution radio observations of NGC 4631: probing the central starburst.
o	CM 67 = [CM69] NGC 4631 67
o	Table 3: <[G99b] SS.s+SSs> N=20.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GA2002]
[GA2002]	(Gyulbudaghian+Akopian, 2002) (Not yet in Simbad)
Write:	<<[GA2002] Puppis A>> <<[GA2002] Puppis AN>>
N:	6+14
Object:	Cloud + Part of Cloud (SIMBAD class: Cloud)
Note:	Clouds in the Association Pup-CMa.
in source:	NAME OB-Association Pup-CMa
Ref:	=2002Ap.....45..432G
by	GYULBUDAGHIAN A.L. , AKOPIAN A.A.
	Astrophysics, 45, 432-437 (2002)
	Velocity distribution of stars in the Pup-CMa association.
o	Table 1: <[GA2002] Puppis A> (Nos A-F), <[GA2002] Puppis AN> (Nos A1-A3, B1-B2, D1-D5, F1-F4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GA2004]
[GA2004]	(Gutierrez+Azzaro, 2004)
Write:	<<[GA2004] NGC 5965aN>>
N:	2
Object:	Satellite G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Photometry of satellite galaxies. Satellite galaxies are ZSFW in SIMBAD, except NGC 5965a1 and a2: The authors found two objects very close (angular distance between them 1".6) and it is unclear if ZSFW is one of the two galaxies or the combination of both.
Ref:	=2004ApJS..155..395G
by	GUTIERREZ C.M. , AZZARO M.
	Astrophys. J., Suppl. Ser., 155, 395-400 (2004)
	The properties of satellite galaxies in external systems. II. Photometry and colors.
o	Table 1: satellites galaxies are ZSFW objects in SIMBAD, except NGC 5965a1 and NGC 5965a2.
o	Table 1: <[GA2004] NGC 5965aN> (Nos a1, a2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GA90]
[GA90]	(Gyulbudaghian+Akopian, 1990)= [GH90] = ([GOA94])
Write:	<<[GA90] 1-NNa>> <<[GA90] 1-NN.N>> <<[GA90] 2-N>> <<[GA90] 3-NN>>
N:	27+6+42
Object:	Radial Syst. + Dk Globule (SIMBAD class: PartofCloud = Part of Cloud)
Note:	1st ref.: Table 1: format '1-NN' (Nos 1-17), radial systems with HII regions. Table 2: format '2-N' (Nos 1-6), radial systems without HII regions. Table 3: format '3-NN' (Nos 1-42), globules in radial systems from T. 1 and 2. 2nd ref.: Radial systems listed in T. 1 of 1st ref., format '1-NNa' and '1-NN.N': Objects 1, 3, 5, 8 are divided into two systems Na and Nb, Two new systems are discovered and called 13.1 and 13.2.
Ref:	=1990Afz....33..395G
by	GYULBUDAGYAN A.L. , AKOPYAN V.A.
	Astrofizika, 33, 395-400 (1990)
	Radial systems of dark globules. I.
o	Table 1: <[GA90] 1-NN> N=17, Table 2: <[GA90] 2-N> N=6, Table 3: <[GA90] 3-NN> N=42
Ref:	=1994Ap.....37..317G
by	GYUL'BUDAGYAN A.L. , OGANYAN G.B., AKHVERDYAN L.G.
	Astrophysics, 37, 317-321 (1994)
	On the connection between radial systems of dark globules and stellar associations.
o	CLN 146 and 148 not in SIMBAD
o	<[GA90] 1-NNa> (Nos 1a-1b, 3a-3b, 5a-5b, 8a-8b), <[GA90] 1-NN.N> (Nos 13.1, 13.2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GAB
GAB	(Groot+Augusteijn+Barziv+)
Write:	<<GAB JHHMMSS+DDMM>>
N:	8
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=8 reference stars used in the photometry of GS Pav.
Ref:	=1998A&A...340L..31G
by	GROOT P.J. , AUGUSTEIJN T., BARZIV O., VAN PARADIJS J.
	Astron. Astrophys., 340, 31-34 (1998)
	The eclipsing cataclysmic variable GS Pavonis: Evidence for disk radius changes.
o	Table 2: <GAB JHHMMSS-DDMM> N=8.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GAB2005]
[GAB2005]	(Grutzbauch+Annibali+Bressan+, 2005)
Write:	<<[GAB2005] NNNN>>
N:	95
Object:	G in Group (SIMBAD class: Galaxy)
Note:	Photometric and spectroscopic observations of the NGC 5328 group at the ESO 3.6 m telescope at La Silla.
in source:	NAME NGC 5328 Group = Klem 28
Ref:	=2005MNRAS.364..146G
by	GRUETZBAUCH R. , ANNIBALI F., BRESSAN A., FOCARDI P., KELM B., RAMPAZZO R., ZEILINGER W.W.
	Mon. Not. R. Astron. Soc., 364, 146-162 (2005)
	Optical properties of the NGC 5328 group of galaxies.
o	Table 1: object 6dF J1354457-285159 = FLASH J135445.64-285158.2 in SIMBAD.
o	Table A1: <[GAB2005] NNNN> N=95.
=E=	Catalogue in electronic form as J/MNRAS/364/146
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GaBoDS
GaBoDS	(Garching-Bonn Deep Survey)
Write:	<<GaBoDS NNNNN>>
N:	1070+565
Object:	G (SIMBAD class: Galaxy)
Note:	Search for U- and B-dropouts in ESO 2.2m telescope archival data
in source:	NAME CDFS
Ref:	=2005A&A...441..905H
by	HILDEBRANDT H. , BOMANS D.J., ERBEN T., SCHNEIDER P., SCHIRMER M., CZOSKE O., DIETRICH J.P., SCHRABBACK T., SIMON P., DETTMAR R.-J., HABERZETTL L., HETTERSCHEIDT M., CORDES O.
	Astron. Astrophys., 441, 905-914 (2005)
	GaBoDS: the Garching-Bonn Deep Survey. III. Lyman-break galaxies in the Chandra Deep Field South.
o	Tables A1, A2: <GaBoDS NNNNN> N=1070+565 among (Nos 171-56730).
=E=	Catalogue in electronic form as J/A+A/441/905
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Gabuzda
Gabuzda	(Gabuzda+)
Write:	<<Gabuzda HHMM+DDd Core>> <<Gabuzda HHMM+DDd KN>> <<Gabuzda HHMM+DDd KNA>> <<Gabuzda HHMM+DDd KN.N>> <<Gabuzda HHMM+DDd KNN>> <<Gabuzda HHMM+DDd Ka>> <<Gabuzda HHMM+DDd XN>> <<Gabuzda HHMM+DDd XNA>> <<Gabuzda HHMM+DDd A>> <<Gabuzda HHMM+DDd AN>>
Object:	Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Structure of 21 BL Lac objects format 'HHMM+DDd', with Ohio J 287 = 0851+202, BL Lac = 2200+420. Maps
Ref:	=1987ApJ...323..536R
by	ROBERTS D.H. , GABUZDA D.C., WARDLE J.F.C.
	Astrophys. J., 323, 536-542 (1987)
	Linear polarization structure of the BL Lacertae object OJ 287 at milliardsecond resolution.
o	<Gabuzda 0851+202 KN> (Nos K1-K2>, <Gabuzda 0851+202 Core> N=1.
Ref:	=1989ApJ...336L..59G
by	GABUZDA D.C. , WARDLE J.F.C., ROBERTS D.H.
	Astrophys. J., 336, 59-62 (1989)
	Superluminal motion in the BL Lacertae object OJ 287.
o	<Gabuzda 0851+202 KN> No. K3 added.
Ref:	=1989ApJ...338..743G
by	GABUZDA D.C. , WARDLE J.F.C., ROBERTS D.H.
	Astrophys. J., 338, 743-751 (1989)
	Linear polarization structure of the BL Lacertae object 0735+178 at milliarcsecond resolution.
o	Table 1: <Gabuzda 0735+178 Core> N=1, <Gabuzda 0735+178 KN> (Nos K1-K2).
Ref:	=1989ApJ...347..701G
by	GABUZDA D.C. , CAWTHORNE T.V., ROBERTS D.H., WARDLE J.F.C.
	Astrophys. J., 347, 701-712 (1989)
	The milliarcsecond polarization structure of six BL Lacertae objects.
o	Table 2: <Gabuzda 0454+844 Core> N=1. Table 3: <Gabuzda 1823+568 Core> N=1, <Gabuzda 1823+568 KN> (Nos K1-K2). Table 4: <Gabuzda 2200+420 C> N=1, <Gabuzda 2200+420 KN> (Nos K1-K2).
Ref:	=1992ApJ...388...40G
by	GABUZDA D.C. , CAWTHORNE T.V., ROBERTS D.H., WARDLE J.F.C.
	Astrophys. J., 388, 40-54 (1992)
	A survey of the milliarcsecond polarization properties of BL Lacertae objects at 5 GHz.
o	Table 2, Figs 1-11: <Gabuzda HHMM+DDd Core> N=11, <Gabuzda 0300+470 KN> (Nos K1-K2), <Gabuzda 0306+102 KN> (Nos K1-K2), <Gabuzda 0754+100 KN> (No. K1), <Gabuzda 0954+658 KN> (Nos K1-K3), <Gabuzda 1219+285 KN> (Nos K1-K4), <Gabuzda 1308+326 KN> (Nos K1-K3), <Gabuzda 1538+149 KN> (No. K1), <Gabuzda 1652+398 KN> (Nos K1-K2), <Gabuzda 1749+701 KN> (Nos K1-K3), <Gabuzda 1803+784 KN> (Nos K1-K2).
Ref:	=1994ApJ...435..128G
by	GABUZDA D.C. , WARDLE J.F.C., ROBERTS D.H., ALLER M.F., ALLER H.D.
	Astrophys. J., 435, 128-139 (1994)
	Unusual evolution in the VLBI structure of 0735+178.
o	Fig.1, 2, Tables 2, 3: <Gabuzda 0735+178 KN> (Nos K3-K6) added, <Gabuzda 0735+178 KN.N> (No. K2.5), <Gabuzda 0735+178 KNA> (No. K0A).
Ref:	=1994ApJ...435..140G
by	GABUZDA D.C. , MULLAN C.M., CAWTHORNE T.V., WARDLE J.F.C., ROBERTS D.H.
	Astrophys. J., 435, 140-161 (1994)
	Evolution of the milliarcsecond total intensity and polarization structures of BL Lacertae objects.
o	Table 2, figs 1-11: <Gabuzda 0300+470 KN> (No. K3), <Gabuzda 0454+844 KN> (Nos K0-K2), <Gabuzda 0954+658 KN> (No. K0), <Gabuzda 1652+398 KN> (No. K0), <Gabuzda 1749+701 KNN> (Nos K01-K02), <Gabuzda 1803+784 KNN> (Nos K01-K03), <Gabuzda 1823+568 KN> (Nos K0, K3), <Gabuzda 2007+777 Core> N=1, <Gabuzda 2007+777 KN> (Nos K1-K5).
Ref:	=1996MNRAS.278..861C
by	CAWTHORNE T.V. , GABUZDA D.C.
	Mon. Not. R. Astron. Soc., 278, 861-868 (1996)
	Milliarcsecond-scale polarization structure in the quasars 3C 279 and 3C 454.3.
o	Table 2: 3C279C2, 3C279C3, 3C279C4. Table 4: 3C 454.3 = PKS 2251+158
o	Table 4: <Gabuzda 2251+158 Core>, <Gabuzda 2251+158 KN> (Nos K1-K7).
Ref:	=1996MNRAS.283..759G
by	GABUZDA D.C. , CAWTHORNE T.V.
	Mon. Not. R. Astron. Soc., 283, 759-776 (1996)
	The parsec-scale polarization structure of nine BL Lacertae objects at λ = 3.6 cm.
o	Table 3, Figs 4-11: <Gabuzda 0454+844 KN> (No. K3), <Gabuzda 0735+178 A> (No. P), <Gabuzda 0851+202 KN> (Nos K4-K5), <Gabuzda 0954+658 KN> (Nos K4-K6), <Gabuzda 1219+285 KN> (Nos K0, K6-K7), <Gabuzda 1219+285 KN.N> (No. 3.5), <Gabuzda 1803+784 KN> (No. K3), <Gabuzda 1803+784 KNA> (Nos K0A-KOB), <Gabuzda 1823+568 KN> (No. K4), <Gabuzda 1823+568 KNA> (Nos K0A), <Gabuzda 2200+420 KN> (No. K3).
Ref:	=1998A&A...333..445G
by	GABUZDA D.C. , KOVALEV Y.Y., KRICHBAUM T.P., ALEF W., KRAUS A., WITZEL A., QUIRRENBACH A.
	Astron. Astrophys., 333, 445-451 (1998)
	VLBI polarization observations of the rapidly variable BL Lacertae object BL 0716+714.
o	Table 2, Figs: <Gabuzda 0716+714 Core> N=1, <Gabuzda 0716+714 CN> (Nos C1-C2), <Gabuzda 0716+714 KN> (Nos K1-K3), <Gabuzda 0716+714 XNA> (Nos X1-X3, X0A).
Ref:	=1999NewAR..43..695P
by	PUSHKAREV A.B. , GABUZDA D.C.
	New Astronomy Reviews, 43, 695-698 (1999)
	Global VLBI polarisation observations of BL Lac objects.
o	Fig 1: <Gabuzda 0003-066 KN> (Nos K1-K4), <Gabuzda 0003-066 Core> N=1. Fig 2: <Gabuzda 1538+149 Ka> (Nos Ka-Kc). Fig 3: <Gabuzda 2254+074 KN> (Nos K1-K5), <Gabuzda 2254+074 Ka> (No. Ka), <Gabuzda 2254+074 Core> N=1.
Ref:	=2000MNRAS.319.1056G
by	GABUZDA D.C. , CAWTHORNE T.V.
	Mon. Not. R. Astron. Soc., 319, 1056-1066 (2000)
	VLBI polarization images of eight compact active galactic nuclei at λ=1.3cm.
o	Table 2: <Gabuzda 1253-055 Core>, <Gabuzda 1253-055 KNA> (Nos K1-K4, K1A-K1C) new. Table 2: <Gabuzda 2200+420 KN> (Nos K4-K5) added.
Ref:	=2000MNRAS.319.1109G
by	GABUZDA D.C. , PUSHKAREV A.B., CAWTHORNE T.V.
	Mon. Not. R. Astron. Soc., 319, 1109-1124 (2000)
	Analysis of λ=6cm VLBI polarization observations of a complete sample of northern BL Lacertae objects.
o	Table 3: <Gabuzda HHMM+DDd Core> N=8, <Gabuzda 0003-066 KN> (Nos K4-K5) added, <Gabuzda 0814+425 KN> (Nos K1-K5), <Gabuzda 0820+225 KNN> (Nos K1-K11), <Gabuzda 0823+033 KN> (Nos K1-K3), <Gabuzda 1334-127 KN> (Nos K1-K3), <Gabuzda 1732+389 KN> (Nos K1-K3), <Gabuzda 2131-021 KN> (Nos K1-K5), <Gabuzda 2155-152 KN> (Nos K, K1)), <Gabuzda 2150+173 KN> (Nos K1-K5).
Ref:	=2001MNRAS.327.1071R
by	REYNOLDS C. , CAWTHORNE T.V., GABUZDA D.C.
	Mon. Not. R. Astron. Soc., 327, 1071-1080 (2001)
	Faraday rotation in the VLBI core of BL Lacertae.
o	Table 2: <Gabuzda 2200+420 KNN> (Nos K8-K11) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GAC2015]
[GAC2015]	(Gunthardt+Aguero+Camperi+, 2015)
Write:	<<[GAC2015] ANN>> <<[GAC2015] ANN-N>>
N:	19
Object:	(MIR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Gemini South T-ReCS MIR observations of N=19 knots in the central region of NGC 253.
in source:	NGC 253
Ref:	=2015AJ....150..139G
by	GUNTHARDT G.I. , AGUERO M.P., CAMPERI J.A., DIAZ R.J., GOMEZ P.L., BOSCH G., SCHIRMER M.
	Astron. J., 150, 139 (2015)
	Uncovering the nucleus candidate for NGC 253.
o	THN = [TH85] N; X-1 = [MGF2010] X-1; IR-NN = [FPA2009] NN.
o	Fig. 6, Table 2: <[GAC2015] ANN-N> (Nos A1, A1-1 to A1-4, A2-A15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GAD2014]
[GAD2014]	(Guennou L.+Adami C.+Durret+, 2014)
Write:	<<[GAD2014] DDD.ddddd+DD.ddddd>> <<[GAD2014] DDD.ddd+DD.ddd>> <<[GAD2014] 326.508+04.41>>
N:	31+27+1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT/FORS2 spectroscopy of N=31+28 galaxies in the field of the RX J1540.8+1445 and GHO 214334+040854 clusters.
in source:	RX J1540.8+1445
in source:	GHO 214334+040854
Ref:	=2014A&A...561A.112G
by	GUENNOU L. , ADAMI C., DURRET F., LIMA NETO G.B., ULMER M.P., CLOWE D., LEBRUN V., MARTINET N., ALLAM S., ANNIS J., BASA S., BENOIST C., BIVIANO A., CAPPI A., CYPRIANO E.S., GAVAZZI R., HALLIDAY C., ILBERT O., JULLO E., JUST D., LIMOUSIN M., MARQUEZ I., MAZURE A., MURPHY K.J., PLANA H., ROSTAGNI F., RUSSEIL D., SCHIRMER M., SLEZAK E., TUCKER D., ZARITSKY D., ZIEGLER B.
	Astron. Astrophys., 561A, 112-112 (2014)
	Structure and substructure analysis of DAFT/FADA galaxy clusters in the [0.4-0.9] redshift range.
o	Table C.2: <[GAD2014] DDD.ddddd+DD.ddddd> N=31, <[GAD2014] DDD.ddd+DD.ddd> N=27, <[GAD2014] 326.508+04.41> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GAD2020]
[GAD2020]	(Ginsburg+Anderson+Dicker+, 2020)
Write:	<<[GAD2020] GLLL.lll+BB.bbb>>
N:	278
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	Green Bank Telescope observations at 3 mm (90 GHz) of N=278 sources, as part of the Green Bank Telescope MUSTANG-2 Galactic Plane survey at 3 mm (90 GHz), MGPS90. The acronym applies only to the sources with S/N>5 and a peak signal at least twice that of the background.
Ref:	=2020ApJS..248...24G
by	GINSBURG A. , ANDERSON L.D., DICKER S., ROMERO C., SVOBODA B., DEVLIN M., GALVAN-MADRID R., INDEBETOUW R., LIU H.B., MASON B., MROCZKOWSKI T., ARMENTROUT W.P., BALLY J., BROGAN C., BUTTERFIELD N., HUNTER T.R., REESE E.D., ROSOLOWSKY E., SARAZIN C., SHIRLEY Y., SIEVERS J., STANCHFIELD S.
	Astrophys. J., Suppl. Ser., 248, 24-24 (2020)
	The MUSTANG Galactic Plane survey (MGPS90) pilot.
o	Table B1: <[GAD2020] GLLL.lll+BB.bbb> N=278.
=E=	Catalogue in electronic form as <J/ApJS/248/24/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GAF2004]
[GAF2004]	(Gallart+Aparicioo+Freedman+, 2004)
Write:	<<[GAF2004] NNNNNN>>
N:	30
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Search for variable star in the Phoenix galaxy. Optical observations at the 100 inch du Pont telescope at Las Campanas Observatory and at the VLT (FORS). Use of ESO NTT and VLT archival data.
in source:	NAME Phe
Ref:	=2004AJ....127.1486G
by	GALLART C. , APARICIO A., FREEDMAN W.L., MADORE B.F., MARTINEZ-DELGADO D., STETSON P.B.
	Astron. J., 127, 1486-1501 (2004)
	The variable-star population in Phoenix: coexistence of anomalous and short-period classical cepheids and detection of RR Lyrae variables.
o	Table 2: <[GAF2004] NNNNNN> N=30 among (Nos 2347-104248)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GAG94]
[GAG94]	(Georgelin+Amram+Georgelin+, 1994)
Write:	<<[GAG94] RCW 94.N>> <<[GAG94] LLL.lll+B.bbb>> <<[GAG94] CO LLL.l+B.b>> <<[GAG94] HA LLL.l+B.b>>
N:	4+27+14+8
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Table 2: N=4 HII region in RCW 94, format 'RCW 94.1' to 'RCW 94.4. Table 4: N=27 radio continuum sources, format 'LLL.lll+B.bbb'. N=8 CO em. sources, format 'CO LLL.l+B.b'. N=14 H-alpha em. sources, format 'HA LLL.l+B.b'. Paper II, see also [LAB92], [GRM96], [RGA98], [GRA2000].
Ref:	=1994A&AS..108..513G
by	GEORGELIN Y.M. , AMRAM P., GEORGELIN Y.P., LE COARER E., MARCELIN M.
	Astron. Astrophys., Suppl. Ser., 108, 513-532 (1994)
	Deep Hα survey of the Milky Way. II. The l=328° area.
o	Table 3: BDMW = [OM80], MF = Muzzio, D = [D72].
o	Table 2: <[GAG94] RCW 94.N> N=4. Table 4: <[GAG94] LLL.lll+B.bbb> N=27, <[GAG94] CO LLL.l+B.b> N=14, <[GAG94] HA LLL.l+B.b> N=8
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Gaia
Gaia	(Gaia)
Write:	<<Gaia -N>> <<Gaia -Na>>
N:	2
Object:	* + Poss. Planet (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Exoplanets and their host stars detected using Gaia photometry.
Ref:	=2022A&A...663A.101P
by	PANAHI A. , ZUCKER S., CLEMENTINI G., AUDARD M., BINNENFELD A., CUSANO F., EVANS D.W., GOMEL R., HOLL B., ILYIN I., JEVARDAT DE FOMBELLE G., MAZEH T., MOWLAVI N., NIENARTOWICZ K., RIMOLDINI L., SHAHAF S., EYER L.
	Astron. Astrophys., 663A, 101-101 (2022)
	The detection of transiting exoplanets by Gaia.
o	<Gaia-Na> (Nos 1-2, 1b, 2b).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Gaia
Gaia	(Gaia sources)
Write:	<<Gaia DRN NNNNNNNNNNNNNNNNNNN>> <<Gaia EDR3 NNNNNNNNNNNNNNNNNNN>>
N:	∼2000000000
Object:	Point Source (SIMBAD class: Star)
Note:	Gaia is an ESA cornerstone mission mapping the point sources on the sky to a magnitude limit of 20.7. Positions are variable due to proper motions which are fundamental elements of the catalogue. The format is made of the number of the data release and the source ID, which contains relevant information of the source (HEALPix) and includes a scheme for the recording of multiple components of a system.
Ref:	=2016A&A...595A...1G
by	GAIA COLLABORATION , PRUSTI T., DE BRUIJNE J.H.J., BROWN A.G.A., VALLENARI A., BABUSIAUX C., BAILER-JONES C.A.L., BASTIAN U., BIERMANN M., EVANS D.W., EYER L., JANSEN F., JORDI C., KLIONER S.A., LAMMERS U., LINDEGREN L., LURI X., MIGNARD F., MILLIGAN D.J., PANEM C., POINSIGNON V., POURBAIX D., RANDICH S., SARRI G., SARTORETTI P., SIDDIQUI H.I., SOUBIRAN C., VALETTE V., VAN LEEUWEN F., WALTON N.A., AERTS C., ARENOU F., CROPPER M., DRIMMEL R., HOG E., KATZ D., LATTANZI M.G., O'MULLANE W., GREBEL E.K., HOLLAND A.D., HUC C., PASSOT X., BRAMANTE L., CACCIARI C., CASTANEDA J., CHAOUL L., CHEEK N., DE ANGELI F., FABRICIUS C., GUERRA R., HERNANDEZ J., JEAN-ANTOINE-PICCOLO A., MASANA E., MESSINEO R., MOWLAVI N., NIENARTOWICZ K., ORDONEZ-BLANCO D., PANUZZO P., PORTELL J., RICHARDS P.J., RIELLO M., SEABROKE G.M., TANGA P., THEVENIN F., TORRA J., ELS S.G., GRACIA-ABRIL G., COMORETTO G., GARCIA-REINALDOS M., LOCK T., MERCIER E., ALTMANN M., ANDRAE R., ASTRAATMADJA T.L., BELLAS-VELIDIS I., BENSON K., BERTHIER J., BLOMME R., BUSSO G., CARRY B., CELLINO A., CLEMENTINI G., COWELL S., CREEVEY O., CUYPERS J., DAVIDSON M., DE RIDDER J., DE TORRES A., DELCHAMBRE L., DELL'ORO A., DUCOURANT C., FREMAT Y., GARCIA-TORRES M., GOSSET E., HALBWACHS J.-L., HAMBLY N.C., HARRISON D.L., HAUSER M., HESTROFFER D., HODGKIN S.T., HUCKLE H.E., HUTTON A., JASNIEWICZ G., JORDAN S., KONTIZAS M., KORN A.J., LANZAFAME A.C., MANTEIGA M., MOITINHO A., MUINONEN K., OSINDE J., PANCINO E., PAUWELS T., PETIT J.-M., RECIO-BLANCO A., ROBIN A.C., SARRO L.M., SIOPIS C., SMITH M., SMITH K.W., SOZZETTI A., THUILLOT W., VAN REEVEN W., VIALA Y., ABBAS U., ABREU ARAMBURU A., ACCART S., AGUADO J.J., ALLAN P.M., ALLASIA W., ALTAVILLA G., ALVAREZ M.A., ALVES J., ANDERSON R.I., ANDREI A.H., ANGLADA VARELA E., ANTICHE E., ANTOJA T., ANTON S., ARCAY B., ATZEI A., AYACHE L., BACH N., BAKER S.G., BALAGUER-NUNEZ L., BARACHE C., BARATA C., BARBIER A., BARBLAN F., BARONI M., BARRADO Y NAVASCUES D., BARROS M., BARSTOW M.A., BECCIANI U., BELLAZZINI M., BELLEI G., BELLO GARCIA A., BELOKUROV V., BENDJOYA P., BERIHUETE A., BIANCHI L., BIENAYME O., BILLEBAUD F., BLAGORODNOVA N., BLANCO-CUARESMA S., BOCH T., BOMBRUN A., BORRACHERO R., BOUQUILLON S., BOURDA G., BOUY H., BRAGAGLIA A., BREDDELS M.A., BROUILLET N., BRUSEMEISTER T., BUCCIARELLI B., BUDNIK F., BURGESS P., BURGON R., BURLACU A., BUSONERO D., BUZZI R., CAFFAU E., CAMBRAS J., CAMPBELL H., CANCELLIERE R., CANTAT-GAUDIN T., CARLUCCI T., CARRASCO J.M., CASTELLANI M., CHARLOT P., CHARNAS J., CHARVET P., CHASSAT F., CHIAVASSA A., CLOTET M., COCOZZA G., COLLINS R.S., COLLINS P., COSTIGAN G., CRIFO F., CROSS N.J.G., CROSTA M., CROWLEY C., DAFONTE C., DAMERDJI Y., DAPERGOLAS A., DAVID P., DAVID M., DE CAT P., DE FELICE F., DE LAVERNY P., DE LUISE F., DE MARCH R., DE MARTINO D., DE SOUZA R., DEBOSSCHER J., DEL POZO E., DELBO M., DELGADO A., DELGADO H.E., DI MARCO F., DI MATTEO P., DIAKITE S., DISTEFANO E., DOLDING C., DOS ANJOS S., DRAZINOS P., DURAN J., DZIGAN Y., ECALE E., EDVARDSSON B., ENKE H., ERDMANN M., ESCOLAR D., ESPINA M., EVANS N.W., EYNARD BONTEMPS G., FABRE C., FABRIZIO M., FAIGLER S., FALCAO A.J., FARRAS CASAS M., FAYE F., FEDERICI L., FEDORETS G., FERNANDEZ-HERNANDEZ J., FERNIQUE P., FIENGA A., FIGUERAS F., FILIPPI F., FINDEISEN K., FONTI A., FOUESNEAU M., FRAILE E., FRASER M., FUCHS J., FURNELL R., GAI M., GALLETI S., GALLUCCIO L., GARABATO D., GARCIA-SEDANO F., GARE P., GAROFALO A., GARRALDA N., GAVRAS P., GERSSEN J., GEYER R., GILMORE G., GIRONA S., GIUFFRIDA G., GOMES M., GONZALEZ-MARCOS A., GONZALEZ-NUNEZ J., GONZALEZ-VIDAL J.J., GRANVIK M., GUERRIER A., GUILLOUT P., GUIRAUD J., GURPIDE A., GUTIERREZ-SANCHEZ R., GUY L.P., HAIGRON R., HATZIDIMITRIOU D., HAYWOOD M., HEITER U., HELMI A., HOBBS D., HOFMANN W., HOLL B., HOLLAND G., HUNT J.A.S., HYPKI A., ICARDI V., IRWIN M., JEVARDAT DE FOMBELLE G., JOFRE P., JONKER P.G., JORISSEN A., JULBE F., KARAMPELAS A., KOCHOSKA A., KOHLEY R., KOLENBERG K., KONTIZAS E., KOPOSOV S.E., KORDOPATIS G., KOUBSKY P., KOWALCZYK A., KRONE-MARTINS A., KUDRYASHOVA M., KULL I., BACHCHAN R.K., LACOSTE-SERIS F., LANZA A.F., LAVIGNE J.-B., LE PONCIN-LAFITTE C., LEBRETON Y., LEBZELTER T., LECCIA S., LECLERC N., LECOEUR-TAIBI I., LEMAITRE V., LENHARDT H., LEROUX F., LIAO S., LICATA E., LINDSTROM H.E.P., LISTER T.A., LIVANOU E., LOBEL A., LOFFLER W., LOPEZ M., LOPEZ-LOZANO A., LORENZ D., LOUREIRO T., MacDONALD I., MAGALHAES FERNANDES T., MANAGAU S., MANN R.G., MANTELET G., MARCHAL O., MARCHANT J.M., MARCONI M., MARIE J., MARINONI S., MARRESE P.M., MARSCHALKO G., MARSHALL D.J., MARTIN-FLEITAS J.M., MARTINO M., MARY N., MATIJEVIC G., MAZEH T., McMILLAN P.J., MESSINA S., MESTRE A., MICHALIK D., MILLAR N.R., MIRANDA B.M.H., MOLINA D., MOLINARO R., MOLINARO M., MOLNAR L., MONIEZ M., MONTEGRIFFO P., MONTEIRO D., MOR R., MORA A., MORBIDELLI R., MOREL T., MORGENTHALER S., MORLEY T., MORRIS D., MULONE A.F., MURAVEVA T., MUSELLA I., NARBONNE J., NELEMANS G., NICASTRO L., NOVAL L., ORDENOVIC C., ORDIERES-MERE J., OSBORNE P., PAGANI C., PAGANO I., PAILLER F., PALACIN H., PALAVERSA L., PARSONS P., PAULSEN T., PECORARO M., PEDROSA R., PENTIKAINEN H., PEREIRA J., PICHON B., PIERSIMONI A.M., PINEAU F.-X., PLACHY E., PLUM G., POUJOULET E., PRSA A., PULONE L., RAGAINI S., RAGO S., RAMBAUX N., RAMOS-LERATE M., RANALLI P., RAUW G., READ A., REGIBO S., RENK F., REYLE C., RIBEIRO R.A., RIMOLDINI L., RIPEPI V., RIVA A., RIXON G., ROELENS M., ROMERO-GOMEZ M., ROWELL N., ROYER F., RUDOLPH A., RUIZ-DERN L., SADOWSKI G., SAGRISTA SELLES T., SAHLMANN J., SALGADO J., SALGUERO E., SARASSO M., SAVIETTO H., SCHNORHK A., SCHULTHEIS M., SCIACCA E., SEGOL M., SEGOVIA J.C., SEGRANSAN D., SERPELL E., SHIH I.-C., SMAREGLIA R., SMART R.L., SMITH C., SOLANO E., SOLITRO F., SORDO R., SORIA NIETO S., SOUCHAY J., SPAGNA A., SPOTO F., STAMPA U., STEELE I.A., STEIDELMULLER H., STEPHENSON C.A., STOEV H., SUESS F.F., SUVEGES M., SURDEJ J., SZABADOS L., SZEGEDI-ELEK E., TAPIADOR D., TARIS F., TAURAN G., TAYLOR M.B., TEIXEIRA R., TERRETT D., TINGLEY B., TRAGER S.C., TURON C., ULLA A., UTRILLA E., VALENTINI G., VAN ELTEREN A., VAN HEMELRYCK E., VAN LEEUWEN M., VARADI M., VECCHIATO A., VELJANOSKI J., VIA T., VICENTE D., VOGT S., VOSS H., VOTRUBA V., VOUTSINAS S., WALMSLEY G., WEILER M., WEINGRILL K., WERNER D., WEVERS T., WHITEHEAD G., WYRZYKOWSKI L., YOLDAS A., ZERJAL M., ZUCKER S., ZURBACH C., ZWITTER T., ALECU A., ALLEN M., ALLENDE PRIETO C., AMORIM A., ANGLADA-ESCUDE G., ARSENIJEVIC V., AZAZ S., BALM P., BECK M., BERNSTEIN H.-H., BIGOT L., BIJAOUI A., BLASCO C., BONFIGLI M., BONO G., BOUDREAULT S., BRESSAN A., BROWN S., BRUNET P.-M., BUNCLARK P., BUONANNO R., BUTKEVICH A.G., CARRET C., CARRION C., CHEMIN L., CHEREAU F., CORCIONE L., DARMIGNY E., DE BOER K.S., DE TEODORO P., DE ZEEUW P.T., DELLE LUCHE C., DOMINGUES C.D., DUBATH P., FODOR F., FREZOULS B., FRIES A., FUSTES D., FYFE D., GALLARDO E., GALLEGOS J., GARDIOL D., GEBRAN M., GOMBOC A., GOMEZ A., GRUX E., GUEGUEN A., HEYROVSKY A., HOAR J., IANNICOLA G., ISASI PARACHE Y., JANOTTO A.-M., JOLIET E., JONCKHEERE A., KEIL R., KIM D.-W., KLAGYIVIK P., KLAR J., KNUDE J., KOCHUKHOV O., KOLKA I., KOS J., KUTKA A., LAINEY V., LEBOUQUIN D., LIU C., LOREGGIA D., MAKAROV V.V., MARSEILLE M.G., MARTAYAN C., MARTINEZ-RUBI O., MASSART B., MEYNADIER F., MIGNOT S., MUNARI U., NGUYEN A.-T., NORDLANDER T., OCVIRK P., O'FLAHERTY K.S., OLIAS SANZ A., ORTIZ P., OSORIO J., OSZKIEWICZ D., OUZOUNIS A., PALMER M., PARK P., PASQUATO E., PELTZER C., PERALTA J., PETURAUD F., PIENILUOMA T., PIGOZZI E., POELS J., PRAT G., PROD'HOMME T., RAISON F., REBORDAO J.M., RISQUEZ D., ROCCA-VOLMERANGE B., ROSEN S., RUIZ-FUERTES M.I., RUSSO F., SEMBAY S., SERRALLER VIZCAINO I., SHORT A., SIEBERT A., SILVA H., SINACHOPOULOS D., SLEZAK E., SOFFEL M., SOSNOWSKA D., STRAIZYS V., TER LINDEN M., TERRELL D., THEIL S., TIEDE C., TROISI L., TSALMANTZA P., TUR D., VACCARI M., VACHIER F., VALLES P., VAN HAMME W., VELTZ L., VIRTANEN J., WALLUT J.-M., WICHMANN R., WILKINSON M.I., ZIAEEPOUR H., ZSCHOCKE S.
	Astron. Astrophys., 595A, 1-1 (2016)
	The Gaia mission.
o	<Gaia DRN NNNNNNNNNNNNNNNNNNN> N about 2 billion.
Ref:	=2016A&A...595A...2G
by	GAIA COLLABORATION , BROWN A.G.A., VALLENARI A., PRUSTI T., DE BRUIJNE J.H.J., MIGNARD F., DRIMMEL R., BABUSIAUX C., BAILER-JONES C.A.L., BASTIAN U., BIERMANN M., EVANS D.W., EYER L., JANSEN F., JORDI C., KATZ D., KLIONER S.A., LAMMERS U., LINDEGREN L., LURI X., O'MULLANE W., PANEM C., POURBAIX D., RANDICH S., SARTORETTI P., SIDDIQUI H.I., SOUBIRAN C., VALETTE V., VAN LEEUWEN F., WALTON N.A., AERTS C., ARENOU F., CROPPER M., HOG E., LATTANZI M.G., GREBEL E.K., HOLLAND A.D., HUC C., PASSOT X., PERRYMAN M., BRAMANTE L., CACCIARI C., CASTANEDA J., CHAOUL L., CHEEK N., DE ANGELI F., FABRICIUS C., GUERRA R., HERNANDEZ J., JEAN-ANTOINE-PICCOLO A., MASANA E., MESSINEO R., MOWLAVI N., NIENARTOWICZ K., ORDONEZ-BLANCO D., PANUZZO P., PORTELL J., RICHARDS P.J., RIELLO M., SEABROKE G.M., TANGA P., THEVENIN F., TORRA J., ELS S.G., GRACIA-ABRIL G., COMORETTO G., GARCIA-REINALDOS M., LOCK T., MERCIER E., ALTMANN M., ANDRAE R., ASTRAATMADJA T.L., BELLAS-VELIDIS I., BENSON K., BERTHIER J., BLOMME R., BUSSO G., CARRY B., CELLINO A., CLEMENTINI G., COWELL S., CREEVEY O., CUYPERS J., DAVIDSON M., DE RIDDER J., DE TORRES A., DELCHAMBRE L., DELL'ORO A., DUCOURANT C., FREMAT Y., GARCIA-TORRES M., GOSSET E., HALBWACHS J.-L., HAMBLY N.C., HARRISON D.L., HAUSER M., HESTROFFER D., HODGKIN S.T., HUCKLE H.E., HUTTON A., JASNIEWICZ G., JORDAN S., KONTIZAS M., KORN A.J., LANZAFAME A.C., MANTEIGA M., MOITINHO A., MUINONEN K., OSINDE J., PANCINO E., PAUWELS T., PETIT J.-M., RECIO-BLANCO A., ROBIN A.C., SARRO L.M., SIOPIS C., SMITH M., SMITH K.W., SOZZETTI A., THUILLOT W., VAN REEVEN W., VIALA Y., ABBAS U., ABREU ARAMBURU A., ACCART S., AGUADO J.J., ALLAN P.M., ALLASIA W., ALTAVILLA G., ALVAREZ M.A., ALVES J., ANDERSON R.I., ANDREI A.H., ANGLADA VARELA E., ANTICHE E., ANTOJA T., ANTON S., ARCAY B., BACH N., BAKER S.G., BALAGUER-NUNEZ L., BARACHE C., BARATA C., BARBIER A., BARBLAN F., BARRADO Y NAVASCUES D., BARROS M., BARSTOW M.A., BECCIANI U., BELLAZZINI M., BELLO GARCIA A., BELOKUROV V., BENDJOYA P., BERIHUETE A., BIANCHI L., BIENAYME O., BILLEBAUD F., BLAGORODNOVA N., BLANCO-CUARESMA S., BOCH T., BOMBRUN A., BORRACHERO R., BOUQUILLON S., BOURDA G., BOUY H., BRAGAGLIA A., BREDDELS M.A., BROUILLET N., BRUSEMEISTER T., BUCCIARELLI B., BURGESS P., BURGON R., BURLACU A., BUSONERO D., BUZZI R., CAFFAU E., CAMBRAS J., CAMPBELL H., CANCELLIERE R., CANTAT-GAUDIN T., CARLUCCI T., CARRASCO J.M., CASTELLANI M., CHARLOT P., CHARNAS J., CHIAVASSA A., CLOTET M., COCOZZA G., COLLINS R.S., COSTIGAN G., CRIFO F., CROSS N.J.G., CROSTA M., CROWLEY C., DAFONTE C., DAMERDJI Y., DAPERGOLAS A., DAVID P., DAVID M., DE CAT P., DE FELICE F., DE LAVERNY P., DE LUISE F., DE MARCH R., DE MARTINO D., DE SOUZA R., DEBOSSCHER J., DEL POZO E., DELBO M., DELGADO A., DELGADO H.E., DI MATTEO P., DIAKITE S., DISTEFANO E., DOLDING C., DOS ANJOS S., DRAZINOS P., DURAN J., DZIGAN Y., EDVARDSSON B., ENKE H., EVANS N.W., EYNARD BONTEMPS G., FABRE C., FABRIZIO M., FAIGLER S., FALCAO A.J., FARRAS CASAS M., FEDERICI L., FEDORETS G., FERNANDEZ-HERNANDEZ J., FERNIQUE P., FIENGA A., FIGUERAS F., FILIPPI F., FINDEISEN K., FONTI A., FOUESNEAU M., FRAILE E., FRASER M., FUCHS J., GAI M., GALLETI S., GALLUCCIO L., GARABATO D., GARCIA-SEDANO F., GAROFALO A., GARRALDA N., GAVRAS P., GERSSEN J., GEYER R., GILMORE G., GIRONA S., GIUFFRIDA G., GOMES M., GONZALEZ-MARCOS A., GONZALEZ-NUNEZ J., GONZALEZ-VIDAL J.J., GRANVIK M., GUERRIER A., GUILLOUT P., GUIRAUD J., GURPIDE A., GUTIERREZ-SANCHEZ R., GUY L.P., HAIGRON R., HATZIDIMITRIOU D., HAYWOOD M., HEITER U., HELMI A., HOBBS D., HOFMANN W., HOLL B., HOLLAND G., HUNT J.A.S., HYPKI A., ICARDI V., IRWIN M., JEVARDAT DE FOMBELLE G., JOFRE P., JONKER P.G., JORISSEN A., JULBE F., KARAMPELAS A., KOCHOSKA A., KOHLEY R., KOLENBERG K., KONTIZAS E., KOPOSOV S.E., KORDOPATIS G., KOUBSKY P., KRONE-MARTINS A., KUDRYASHOVA M., KULL I., BACHCHAN R.K., LACOSTE-SERIS F., LANZA A.F., LAVIGNE J.-B., LE PONCIN-LAFITTE C., LEBRETON Y., LEBZELTER T., LECCIA S., LECLERC N., LECOEUR-TAIBI I., LEMAITRE V., LENHARDT H., LEROUX F., LIAO S., LICATA E., LINDSTROM H.E.P., LISTER T.A., LIVANOU E., LOBEL A., LOFFLER W., LOPEZ M., LORENZ D., MacDONALD I., MAGALHAES FERNANDES T., MANAGAU S., MANN R.G., MANTELET G., MARCHAL O., MARCHANT J.M., MARCONI M., MARINONI S., MARRESE P.M., MARSCHALKO G., MARSHALL D.J., MARTIN-FLEITAS J.M., MARTINO M., MARY N., MATIJEVIC G., MAZEH T., McMILLAN P.J., MESSINA S., MICHALIK D., MILLAR N.R., MIRANDA B.M.H., MOLINA D., MOLINARO R., MOLINARO M., MOLNAR L., MONIEZ M., MONTEGRIFFO P., MOR R., MORA A., MORBIDELLI R., MOREL T., MORGENTHALER S., MORRIS D., MULONE A.F., MURAVEVA T., MUSELLA I., NARBONNE J., NELEMANS G., NICASTRO L., NOVAL L., ORDENOVIC C., ORDIERES-MERE J., OSBORNE P., PAGANI C., PAGANO I., PAILLER F., PALACIN H., PALAVERSA L., PARSONS P., PECORARO M., PEDROSA R., PENTIKAINEN H., PICHON B., PIERSIMONI A.M., PINEAU F.-X., PLACHY E., PLUM G., POUJOULET E., PRSA A., PULONE L., RAGAINI S., RAGO S., RAMBAUX N., RAMOS-LERATE M., RANALLI P., RAUW G., READ A., REGIBO S., REYLE C., RIBEIRO R.A., RIMOLDINI L., RIPEPI V., RIVA A., RIXON G., ROELENS M., ROMERO-GOMEZ M., ROWELL N., ROYER F., RUIZ-DERN L., SADOWSKI G., SAGRISTA SELLES T., SAHLMANN J., SALGADO J., SALGUERO E., SARASSO M., SAVIETTO H., SCHULTHEIS M., SCIACCA E., SEGOL M., SEGOVIA J.C., SEGRANSAN D., SHIH I.-C., SMAREGLIA R., SMART R.L., SOLANO E., SOLITRO F., SORDO R., SORIA NIETO S., SOUCHAY J., SPAGNA A., SPOTO F., STAMPA U., STEELE I.A., STEIDELMULLER H., STEPHENSON C.A., STOEV H., SUESS F.F., SUVEGES M., SURDEJ J., SZABADOS L., SZEGEDI-ELEK E., TAPIADOR D., TARIS F., TAURAN G., TAYLOR M.B., TEIXEIRA R., TERRETT D., TINGLEY B., TRAGER S.C., TURON C., ULLA A., UTRILLA E., VALENTINI G., VAN ELTEREN A., VAN HEMELRYCK E., VAN LEEUWEN M., VARADI M., VECCHIATO A., VELJANOSKI J., VIA T., VICENTE D., VOGT S., VOSS H., VOTRUBA V., VOUTSINAS S., WALMSLEY G., WEILER M., WEINGRILL K., WEVERS T., WYRZYKOWSKI L., YOLDAS A., ZERJAL M., ZUCKER S., ZURBACH C., ZWITTER T., ALECU A., ALLEN M., ALLENDE PRIETO C., AMORIM A., ANGLADA-ESCUDE G., ARSENIJEVIC V., AZAZ S., BALM P., BECK M., BERNSTEIN H.-H., BIGOT L., BIJAOUI A., BLASCO C., BONFIGLI M., BONO G., BOUDREAULT S., BRESSAN A., BROWN S., BRUNET P.-M., BUNCLARK P., BUONANNO R., BUTKEVICH A.G., CARRET C., CARRION C., CHEMIN L., CHEREAU F., CORCIONE L., DARMIGNY E., DE BOER K.S., DE TEODORO P., DE ZEEUW P.T., DELLE LUCHE C., DOMINGUES C.D., DUBATH P., FODOR F., FREZOULS B., FRIES A., FUSTES D., FYFE D., GALLARDO E., GALLEGOS J., GARDIOL D., GEBRAN M., GOMBOC A., GOMEZ A., GRUX E., GUEGUEN A., HEYROVSKY A., HOAR J., IANNICOLA G., ISASI PARACHE Y., JANOTTO A.-M., JOLIET E., JONCKHEERE A., KEIL R., KIM D.-W., KLAGYIVIK P., KLAR J., KNUDE J., KOCHUKHOV O., KOLKA I., KOS J., KUTKA A., LAINEY V., LEBOUQUIN D., LIU C., LOREGGIA D., MAKAROV V.V., MARSEILLE M.G., MARTAYAN C., MARTINEZ-RUBI O., MASSART B., MEYNADIER F., MIGNOT S., MUNARI U., NGUYEN A.-T., NORDLANDER T., OCVIRK P., O'FLAHERTY K.S., OLIAS SANZ A., ORTIZ P., OSORIO J., OSZKIEWICZ D., OUZOUNIS A., PALMER M., PARK P., PASQUATO E., PELTZER C., PERALTA J., PETURAUD F., PIENILUOMA T., PIGOZZI E., POELS J., PRAT G., PROD'HOMME T., RAISON F., REBORDAO J.M., RISQUEZ D., ROCCA-VOLMERANGE B., ROSEN S., RUIZ-FUERTES M.I., RUSSO F., SEMBAY S., SERRALLER VIZCAINO I., SHORT A., SIEBERT A., SILVA H., SINACHOPOULOS D., SLEZAK E., SOFFEL M., SOSNOWSKA D., STRAIZYS V., TER LINDEN M., TERRELL D., THEIL S., TIEDE C., TROISI L., TSALMANTZA P., TUR D., VACCARI M., VACHIER F., VALLES P., VAN HAMME W., VELTZ L., VIRTANEN J., WALLUT J.-M., WICHMANN R., WILKINSON M.I., ZIAEEPOUR H., ZSCHOCKE S.
	Astron. Astrophys., 595A, 2-2 (2016)
	Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties.
o	<Gaia DR1 NNNNNNNNNNNNNNNNNNN> N=1142679769.
Ref:	=2018A&A...616A...1G
by	GAIA COLLABORATION , BROWN A.G.A., VALLENARI A., PRUSTI T., DE BRUIJNE J.H.J., BABUSIAUX C., BAILER-JONES C.A.L., BIERMANN M., EVANS D.W., EYER L., JANSEN F., JORDI C., KLIONER S.A., LAMMERS U., LINDEGREN L., LURI X., MIGNARD F., PANEM C., POURBAIX D., RANDICH S., SARTORETTI P., SIDDIQUI H.I., SOUBIRAN C., VAN LEEUWEN F., WALTON N.A., ARENOU F., BASTIAN U., CROPPER M., DRIMMEL R., KATZ D., LATTANZI M.G., BAKKER J., CACCIARI C., CASTANEDA J., CHAOUL L., CHEEK N., DE ANGELI F., FABRICIUS C., GUERRA R., HOLL B., MASANA E., MESSINEO R., MOWLAVI N., NIENARTOWICZ K., PANUZZO P., PORTELL J., RIELLO M., SEABROKE G.M., TANGA P., THEVENIN F., GRACIA-ABRIL G., COMORETTO G., GARCIA-REINALDOS M., TEYSSIER D., ALTMANN M., ANDRAE R., AUDARD M., BELLAS-VELIDIS I., BENSON K., BERTHIER J., BLOMME R., BURGESS P., BUSSO G., CARRY B., CELLINO A., CLEMENTINI G., CLOTET M., CREEVEY O., DAVIDSON M., DE RIDDER J., DELCHAMBRE L., DELL'ORO A., DUCOURANT C., FERNANDEZ-HERNANDEZ J., FOUESNEAU M., FREMAT Y., GALLUCCIO L., GARCIA-TORRES M., GONZALEZ-NUNEZ J., GONZALEZ-VIDAL J.J., GOSSET E., GUY L.P., HALBWACHS J.-L., HAMBLY N.C., HARRISON D.L., HERNANDEZ J., HESTROFFER D., HODGKIN S.T., HUTTON A., JASNIEWICZ G., JEAN-ANTOINE-PICCOLO A., JORDAN S., KORN A.J., KRONE-MARTINS A., LANZAFAME A.C., LEBZELTER T., LOFFLER W., MANTEIGA M., MARRESE P.M., MARTIN-FLEITAS J.M., MOITINHO A., MORA A., MUINONEN K., OSINDE J., PANCINO E., PAUWELS T., PETIT J.-M., RECIO-BLANCO A., RICHARDS P.J., RIMOLDINI L., ROBIN A.C., SARRO L.M., SIOPIS C., SMITH M., SOZZETTI A., SUVEGES M., TORRA J., VAN REEVEN W., ABBAS U., ABREU ARAMBURU A., ACCART S., AERTS C., ALTAVILLA G., ALVAREZ M.A., ALVAREZ R., ALVES J., ANDERSON R.I., ANDREI A.H., ANGLADA VARELA E., ANTICHE E., ANTOJA T., ARCAY B., ASTRAATMADJA T.L., BACH N., BAKER S.G., BALAGUER-NUNEZ L., BALM P., BARACHE C., BARATA C., BARBATO D., BARBLAN F., BARKLEM P.S., BARRADO D., BARROS M., BARSTOW M.A., BARTHOLOME MUNOZ S., BASSILANA J.-L., BECCIANI U., BELLAZZINI M., BERIHUETE A., BERTONE S., BIANCHI L., BIENAYME O., BLANCO-CUARESMA S., BOCH T., BOECHE C., BOMBRUN A., BORRACHERO R., BOSSINI D., BOUQUILLON S., BOURDA G., BRAGAGLIA A., BRAMANTE L., BREDDELS M.A., BRESSAN A., BROUILLET N., BRUSEMEISTER T., BRUGALETTA E., BUCCIARELLI B., BURLACU A., BUSONERO D., BUTKEVICH A.G., BUZZI R., CAFFAU E., CANCELLIERE R., CANNIZZARO G., CANTAT-GAUDIN T., CARBALLO R., CARLUCCI T., CARRASCO J.M., CASAMIQUELA L., CASTELLANI M., CASTRO-GINARD A., CHARLOT P., CHEMIN L., CHIAVASSA A., COCOZZA G., COSTIGAN G., COWELL S., CRIFO F., CROSTA M., CROWLEY C., CUYPERS J., DAFONTE C., DAMERDJI Y., DAPERGOLAS A., DAVID P., DAVID M., DE LAVERNY P., DE LUISE F., DE MARCH R., DE MARTINO D., DE SOUZA R., DE TORRES A., DEBOSSCHER J., DEL POZO E., DELBO M., DELGADO A., DELGADO H.E., DI MATTEO P., DIAKITE S., DIENER C., DISTEFANO E., DOLDING C., DRAZINOS P., DURAN J., EDVARDSSON B., ENKE H., ERIKSSON K., ESQUEJ P., EYNARD BONTEMPS G., FABRE C., FABRIZIO M., FAIGLER S., FALCAO A.J., FARRAS CASAS M., FEDERICI L., FEDORETS G., FERNIQUE P., FIGUERAS F., FILIPPI F., FINDEISEN K., FONTI A., FRAILE E., FRASER M., FREZOULS B., GAI M., GALLETI S., GARABATO D., GARCIA-SEDANO F., GAROFALO A., GARRALDA N., GAVEL A., GAVRAS P., GERSSEN J., GEYER R., GIACOBBE P., GILMORE G., GIRONA S., GIUFFRIDA G., GLASS F., GOMES M., GRANVIK M., GUEGUEN A., GUERRIER A., GUIRAUD J., GUTIERREZ-SANCHEZ R., HAIGRON R., HATZIDIMITRIOU D., HAUSER M., HAYWOOD M., HEITER U., HELMI A., HEU J., HILGER T., HOBBS D., HOFMANN W., HOLLAND G., HUCKLE H.E., HYPKI A., ICARDI V., JANSSEN K., JEVARDAT DE FOMBELLE G., JONKER P.G., JUHASZ A.L., JULBE F., KARAMPELAS A., KEWLEY A., KLAR J., KOCHOSKA A., KOHLEY R., KOLENBERG K., KONTIZAS M., KONTIZAS E., KOPOSOV S.E., KORDOPATIS G., KOSTRZEWA-RUTKOWSKA Z., KOUBSKY P., LAMBERT S., LANZA A.F., LASNE Y., LAVIGNE J.-B., LE FUSTEC Y., LE PONCIN-LAFITTE C., LEBRETON Y., LECCIA S., LECLERC N., LECOEUR-TAIBI I., LENHARDT H., LEROUX F., LIAO S., LICATA E., LINDSTROM H.E.P., LISTER T.A., LIVANOU E., LOBEL A., LOPEZ M., MANAGAU S., MANN R.G., MANTELET G., MARCHAL O., MARCHANT J.M., MARCONI M., MARINONI S., MARSCHALKO G., MARSHALL D.J., MARTINO M., MARTON G., MARY N., MASSARI D., MATIJEVIC G., MAZEH T., McMILLAN P.J., MESSINA S., MICHALIK D., MILLAR N.R., MOLINA D., MOLINARO R., MOLNAR L., MONTEGRIFFO P., MOR R., MORBIDELLI R., MOREL T., MORRIS D., MULONE A.F., MURAVEVA T., MUSELLA I., NELEMANS G., NICASTRO L., NOVAL L., O'MULLANE W., ORDENOVIC C., ORDONEZ-BLANCO D., OSBORNE P., PAGANI C., PAGANO I., PAILLER F., PALACIN H., PALAVERSA L., PANAHI A., PAWLAK M., PIERSIMONI A.M., PINEAU F.-X., PLACHY E., PLUM G., POGGIO E., POUJOULET E., PRSA A., PULONE L., RACERO E., RAGAINI S., RAMBAUX N., RAMOS-LERATE M., REGIBO S., REYLE C., RICLET F., RIPEPI V., RIVA A., RIVARD A., RIXON G., ROEGIERS T., ROELENS M., ROMERO-GOMEZ M., ROWELL N., ROYER F., RUIZ-DERN L., SADOWSKI G., SAGRISTA SELLES T., SAHLMANN J., SALGADO J., SALGUERO E., SANNA N., SANTANA-ROS T., SARASSO M., SAVIETTO H., SCHULTHEIS M., SCIACCA E., SEGOL M., SEGOVIA J.C., SEGRANSAN D., SHIH I.-C., SILTALA L., SILVA A.F., SMART R.L., SMITH K.W., SOLANO E., SOLITRO F., SORDO R., SORIA NIETO S., SOUCHAY J., SPAGNA A., SPOTO F., STAMPA U., STEELE I.A., STEIDELMULLER H., STEPHENSON C.A., STOEV H., SUESS F.F., SURDEJ J., SZABADOS L., SZEGEDI-ELEK E., TAPIADOR D., TARIS F., TAURAN G., TAYLOR M.B., TEIXEIRA R., TERRETT D., TEYSSANDIER P., THUILLOT W., TITARENKO A., TORRA CLOTET F., TURON C., ULLA A., UTRILLA E., UZZI S., VAILLANT M., VALENTINI G., VALETTE V., VAN ELTEREN A., VAN HEMELRYCK E., VAN LEEUWEN M., VASCHETTO M., VECCHIATO A., VELJANOSKI J., VIALA Y., VICENTE D., VOGT S., VON ESSEN C., VOSS H., VOTRUBA V., VOUTSINAS S., WALMSLEY G., WEILER M., WERTZ O., WEVERS T., WYRZYKOWSKI L., YOLDAS A., ZERJAL M., ZIAEEPOUR H., ZOREC J., ZSCHOCKE S., ZUCKER S., ZURBACH C., ZWITTER T.
	Astron. Astrophys., 616A, 1-1 (2018)
	Gaia Data Release 2. Summary of the contents and survey properties.
o	<Gaia DR2 NNNNNNNNNNNNNNNNNNN> N=1692919135.
Ref:	=2021A&A...649A...1G
by	GAIA COLLABORATION , BROWN A.G.A., VALLENARI A., PRUSTI T., DE BRUIJNE J.H.J., BABUSIAUX C., BIERMANN M., CREEVEY O.L., EVANS D.W., EYER L., HUTTON A., JANSEN F., JORDI C., KLIONER S.A., LAMMERS U., LINDEGREN L., LURI X., MIGNARD F., PANEM C., POURBAIX D., RANDICH S., SARTORETTI P., SOUBIRAN C., WALTON N.A., ARENOU F., BAILER-JONES C.A.L., BASTIAN U., CROPPER M., DRIMMEL R., KATZ D., LATTANZI M.G., VAN LEEUWEN F., BAKKER J., CACCIARI C., CASTANEDA J., DE ANGELI F., DUCOURANT C., FABRICIUS C., FOUESNEAU M., FREMAT Y., GUERRA R., GUERRIER A., GUIRAUD J., JEAN-ANTOINE-PICCOLO A., MASANA E., MESSINEO R., MOWLAVI N., NICOLAS C., NIENARTOWICZ K., PAILLER F., PANUZZO P., RICLET F., ROUX W., SEABROKE G.M., SORDO R., TANGA P., THEVENIN F., GRACIA-ABRIL G., PORTELL J., TEYSSIER D., ALTMANN M., ANDRAE R., BELLAS-VELIDIS I., BENSON K., BERTHIER J., BLOMME R., BRUGALETTA E., BURGESS P.W., BUSSO G., CARRY B., CELLINO A., CHEEK N., CLEMENTINI G., DAMERDJI Y., DAVIDSON M., DELCHAMBRE L., DELL'ORO A., FERNANDEZ-HERNANDEZ J., GALLUCCIO L., GARCIA-LARIO P., GARCIA-REINALDOS M., GONZALEZ-NUNEZ J., GOSSET E., HAIGRON R., HALBWACHS J.-L., HAMBLY N.C., HARRISON D.L., HATZIDIMITRIOU D., HEITER U., HERNANDEZ J., HESTROFFER D., HODGKIN S.T., HOLL B., JANSSEN K., JEVARDAT DE FOMBELLE G., JORDAN S., KRONE-MARTINS A., LANZAFAME A.C., LOFFLER W., LORCA A., MANTEIGA M., MARCHAL O., MARRESE P.M., MOITINHO A., MORA A., MUINONEN K., OSBORNE P., PANCINO E., PAUWELS T., PETIT J.-M., RECIO-BLANCO A., RICHARDS P.J., RIELLO M., RIMOLDINI L., ROBIN A.C., ROEGIERS T., RYBIZKI J., SARRO L.M., SIOPIS C., SMITH M., SOZZETTI A., ULLA A., UTRILLA E., VAN LEEUWEN M., VAN REEVEN W., ABBAS U., ABREU ARAMBURU A., ACCART S., AERTS C., AGUADO J.J., AJAJ M., ALTAVILLA G., ALVAREZ M.A., ALVAREZ CID-FUENTES J., ALVES J., ANDERSON R.I., ANGLADA VARELA E., ANTOJA T., AUDARD M., BAINES D., BAKER S.G., BALAGUER-NUNEZ L., BALBINOT E., BALOG Z., BARACHE C., BARBATO D., BARROS M., BARSTOW M.A., BARTOLOME S., BASSILANA J.-L., BAUCHET N., BAUDESSON-STELLA A., BECCIANI U., BELLAZZINI M., BERNET M., BERTONE S., BIANCHI L., BLANCO-CUARESMA S., BOCH T., BOMBRUN A., BOSSINI D., BOUQUILLON S., BRAGAGLIA A., BRAMANTE L., BREEDT E., BRESSAN A., BROUILLET N., BUCCIARELLI B., BURLACU A., BUSONERO D., BUTKEVICH A.G., BUZZI R., CAFFAU E., CANCELLIERE R., CANOVAS H., CANTAT-GAUDIN T., CARBALLO R., CARLUCCI T., CARNERERO M.I., CARRASCO J.M., CASAMIQUELA L., CASTELLANI M., CASTRO-GINARD A., CASTRO SAMPOL P., CHAOUL L., CHARLOT P., CHEMIN L., CHIAVASSA A., CIONI M.-R.L., COMORETTO G., COOPER W.J., CORNEZ T., COWELL S., CRIFO F., CROSTA M., CROWLEY C., DAFONTE C., DAPERGOLAS A., DAVID M., DAVID P., DE LAVERNY P., DE LUISE F., DE MARCH R., DE RIDDER J., DE SOUZA R., DE TEODORO P., DE TORRES A., DEL PELOSO E.F., DEL POZO E., DELBO M., DELGADO A., DELGADO H.E., DELISLE J.-B., DI MATTEO P., DIAKITE S., DIENER C., DISTEFANO E., DOLDING C., EAPPACHEN D., EDVARDSSON B., ENKE H., ESQUEJ P., FABRE C., FABRIZIO M., FAIGLER S., FEDORETS G., FERNIQUE P., FIENGA A., FIGUERAS F., FOURON C., FRAGKOUDI F., FRAILE E., FRANKE F., GAI M., GARABATO D., GARCIA-GUTIERREZ A., GARCIA-TORRES M., GAROFALO A., GAVRAS P., GERLACH E., GEYER R., GIACOBBE P., GILMORE G., GIRONA S., GIUFFRIDA G., GOMEL R., GOMEZ A., GONZALEZ-SANTAMARIA I., GONZALEZ-VIDAL J.J., GRANVIK M., GUTIERREZ-SANCHEZ R., GUY L.P., HAUSER M., HAYWOOD M., HELMI A., HIDALGO S.L., HILGER T., HLADCZUK N., HOBBS D., HOLLAND G., HUCKLE H.E., JASNIEWICZ G., JONKER P.G., JUARISTI CAMPILLO J., JULBE F., KARBEVSKA L., KERVELLA P., KHANNA S., KOCHOSKA A., KONTIZAS M., KORDOPATIS G., KORN A.J., KOSTRZEWA-RUTKOWSKA Z., KRUSZYNSKA K., LAMBERT S., LANZA A.F., LASNE Y., LE CAMPION J.-F., LE FUSTEC Y., LEBRETON Y., LEBZELTER T., LECCIA S., LECLERC N., LECOEUR-TAIBI I., LIAO S., LICATA E., LINDSTROM E.P., LISTER T.A., LIVANOU E., LOBEL A., MADRERO PARDO P., MANAGAU S., MANN R.G., MARCHANT J.M., MARCONI M., MARCOS SANTOS M.M.S., MARINONI S., MAROCCO F., MARSHALL D.J., MARTIN POLO L., MARTIN-FLEITAS J.M., MASIP A., MASSARI D., MASTROBUONO-BATTISTI A., MAZEH T., McMILLAN P.J., MESSINA S., MICHALIK D., MILLAR N.R., MINTS A., MOLINA D., MOLINARO R., MOLNAR L., MONTEGRIFFO P., MOR R., MORBIDELLI R., MOREL T., MORRIS D., MULONE A.F., MUNOZ D., MURAVEVA T., MURPHY C.P., MUSELLA I., NOVAL L., ORDENOVIC C., ORRU G., OSINDE J., PAGANI C., PAGANO I., PALAVERSA L., PALICIO P.A., PANAHI A., PAWLAK M., PENALOSA ESTELLER X., PENTTILA A., PIERSIMONI A.M., PINEAU F.-X., PLACHY E., PLUM G., POGGIO E., PORETTI E., POUJOULET E., PRSA A., PULONE L., RACERO E., RAGAINI S., RAINER M., RAITERI C.M., RAMBAUX N., RAMOS P., RAMOS-LERATE M., RE FIORENTIN P., REGIBO S., REYLE C., RIPEPI V., RIVA A., RIXON G., ROBICHON N., ROBIN C., ROELENS M., ROHRBASSER L., ROMERO-GOMEZ M., ROWELL N., ROYER F., RYBICKI K.A., SADOWSKI G., SAGRISTA SELLES A., SAHLMANN J., SALGADO J., SALGUERO E., SAMARAS N., SANCHEZ GIMENEZ V., SANNA N., SANTOVENA R., SARASSO M., SCHULTHEIS M., SCIACCA E., SEGOL M., SEGOVIA J.C., SEGRANSAN D., SEMEUX D., SHAHAF S., SIDDIQUI H.I., SIEBERT A., SILTALA L., SLEZAK E., SMART R.L., SOLANO E., SOLITRO F., SOUAMI D., SOUCHAY J., SPAGNA A., SPOTO F., STEELE I.A., STEIDELMULLER H., STEPHENSON C.A., SUVEGES M., SZABADOS L., SZEGEDI-ELEK E., TARIS F., TAURAN G., TAYLOR M.B., TEIXEIRA R., THUILLOT W., TONELLO N., TORRA F., TORRA J., TURON C., UNGER N., VAILLANT M., VAN DILLEN E., VANEL O., VECCHIATO A., VIALA Y., VICENTE D., VOUTSINAS S., WEILER M., WEVERS T., WYRZYKOWSKI L., YOLDAS A., YVARD P., ZHAO H., ZOREC J., ZUCKER S., ZURBACH C., ZWITTER T.
	Astron. Astrophys., 649A, 1-1 (2021)
	Gaia Early Data Release 3. Summary of the contents and survey properties.
o	See also 2020yCat.1350....0G
o	(Erratum) erratum vol. 650, art. C3 (2021)
o	<Gaia EDR3 NNNNNNNNNNNNNNNNNNN> N=1811709771. ESA
=E=	Catalogue in electronic form as <I/337/>
=E=	Catalogue in electronic form as <I/345/>
=E=	Catalogue in electronic form as <I/350/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: Gaia
Gaia	(Gaia)
Write:	<<Gaia YYaaa>>
Object:	Transient (SIMBAD class: Transient = Transient Event)
Note:	Transients detected by the Gaia Photometric Science Alerts programme. See http://gsaweb.ast.cam.ac.uk/alerts/home
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Gaia
Gaia	(Gaia)
*****	Avoid the usage of Gaia, prefer [KBT2017]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Gaia
Gaia	(Gaia)
*****	Avoid the usage of Gaia, prefer [MIM2018]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GAK2002]
[GAK2002]	(Gaensler+Arons+Kaspi+, 2002) (Not yet in Simbad)
Write:	<<[GAK2002] RCW 89 A>> <<[GAK2002] PSR 1509+58 N>>
N:	6+6
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	CXO observations of the field around RCW 89 and PSR 1509+58.
Ref:	=2002ApJ...569..878G
by	GAENSLER B.M. , ARONS J., KASPI V.M., PIVOVAROFF M.J., KAWAI N., TAMURA K.
	Astrophys. J., 569, 878-893 (2002)
	Chandra imaging of the X-ray nebula powered by pulsar B1509-58.
o	Fig.2: <[GAK2002] RCW 89 A> (Nos A-F). Fig.5: <[GAK2002] PSR 1509+58 N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Gal
Gal	(Galactic coord.)
Write:	<<GAL LLL+BB>> <<GAL LLL.l+BB.b>> <<GAL LLL+BB.bb>> <<GAL LLL.ll+BB.bb>>
Object:	Unknown (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Systematic designation. In SIMBAD only
Details on Acronym: GAL
GAL	(Holden+Franx+Illingworth+, 2009)
Note:	Keck II DEIMOS observations of Cl 1226+33.
Details on Acronym: [GAL2014]
[GAL2014]	(Gaidos+Anderson+Lepine+, 2014)
Write:	<<[GAL2014] JHHMMm+DDMM>>
N:	80 (SIMBAD class: Star)
Note:	Observations of N=80 stars in a search for transiting Neptune-sized planets. Use of WASP-North survey data.
Ref:	=2014MNRAS.437.3133G
by	GAIDOS E. , ANDERSON D.R., LEPINE S., COLON K.D., MARAVELIAS G., NARITA N., CHANG E., BEYER J., FUKUI A., ARMSTRONG J.D., ZEZAS A., FULTON B.J., MANN A.W., WEST R.G., FAEDI F.
	Mon. Not. R. Astron. Soc., 437, 3133-3143 (2014)
	Trawling for transits in a sea of noise: a search for exoplanets by analysis of WASP optical light curves and follow-up (SEAWOLF).
o	GJ 3740b is a misprint for GJ 3470b.
o	Table 2: <[GAL2014] JHHMMm+DDMM> N=80.
=E=	Catalogue in electronic form as J/MNRAS/437/3133
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GALAH
GALAH	(Galactic Archeology with HERMES)
Write:	<<GALAH NNNNNNN>> <<GALAH NNNNNNNNNNNNNNN>>
N:	11320+9860+342682+588571
Object:	* (SIMBAD class: Star)
Note:	AAT 3.9m telescope HERMES observations as part of the Galactic Archeology with HERMES (GALAH) survey, a massive observational project to trace the Milky Way's history of star formation, chemical enrichment, stellar migration, and minor mergers. Use of 2MASS, APASS, UCAC4, K2-HERMES, TESS-HERMES data. For more information, visit: https://galah-survey.org/ 2017MNRAS.465.3203M (DR1, format NNNNNNN): N=9860 2018MNRAS.478.4513B (DR2, format NNNNNNNNNNNNNNN): N=342682 2021MNRAS.506..150B (DR3, format NNNNNNNNNNNNNNN): N=588571
Ref:	=2017ApJS..228...24T
by	TRAVEN G. , MATIJEVIC G., ZWITTER T., ZERJAL M., KOS J., ASPLUND M., BLAND-HAWTHORN J., CASEY A.R., DE SILVA G., FREEMAN K., LIN J., MARTELL S.L., SCHLESINGER K.J., SHARMA S., SIMPSON J.D., ZUCKER D.B., ANGUIANO B., DA COSTA G., DUONG L., HORNER J., HYDE E.A., KAFLE P.R., MUNARI U., NATAF D., NAVIN C.A., REID W., TING Y.-S.
	Astrophys. J., Suppl. Ser., 228, 24-24 (2017)
	The GALAH survey: classification and diagnostics with t-SNE reduction of spectral information.
o	Table 4: <GALAH NNNNNNN> N=11320 among (Nos 0-9520722).
Ref:	=2017MNRAS.465.3203M
by	MARTELL S.L. , SHARMA S., BUDER S., DUONG L., SCHLESINGER K.J., SIMPSON J., LIND K., NESS M., MARSHALL J.P., ASPLUND M., BLAND-HAWTHORN J., CASEY A.R., DE SILVA G., FREEMAN K.C., KOS J., LIN J., ZUCKER D.B., ZWITTER T., ANGUIANO B., BACIGALUPO C., CAROLLO D., CASAGRANDE L., DA COSTA G.S., HORNER J., HUBER D., HYDE E.A., KAFLE P.R., LEWIS G.F., NATAF D., NAVIN C.A., STELLO D., TINNEY C.G., WATSON F.G., WITTENMYER R.
	Mon. Not. R. Astron. Soc., 465, 3203-3219 (2017)
	The GALAH survey: observational overview and Gaia DR1 companion.
o	Table 3: <GALAH NNNNNNNN> N=9860 among (Nos 22245-6392361).
Ref:	=2018MNRAS.478.4513B
by	BUDER S. , ASPLUND M., DUONG L., KOS J., LIND K., NESS M.K., SHARMA S., BLAND-HAWTHORN J., CASEY A.R., DE SILVA G.M., D'ORAZI V., FREEMAN K.C., LEWIS G.F., LIN J., MARTELL S.L., SCHLESINGER K.J., SIMPSON J.D., ZUCKER D.B., ZWITTER T., AMARSI A.M., ANGUIANO B., CAROLLO D., CASAGRANDE L., COTAR K., COTTRELL P.L., DA COSTA G., GAO X.D., HAYDEN M.R., HORNER J., IRELAND M.J., KAFLE P.R., MUNARI U., NATAF D.M., NORDLANDER T., STELLO D., TING Y.-S., TRAVEN G., WATSON F., WITTENMYER R.A., WYSE R.F.G., YONG D., ZINN J.C., ZERJAL M., (The GALAH Collaboration)
	Mon. Not. R. Astron. Soc., 478, 4513-4552 (2018)
	The GALAH Survey: second data release.
o	<GALAH NNNNNNNNNNNNNNN> N=342682.
Ref:	=2021MNRAS.506..150B
by	BUDER S. , SHARMA S., KOS J., AMARSI A.M., NORDLANDER T., LIND K., MARTELL S.L., ASPLUND M., BLAND-HAWTHORN J., CASEY A.R., DE SILVA G.M., D'ORAZI V., FREEMAN K.C., HAYDEN M.R., LEWIS G.F., LIN J., SCHLESINGER K.J., SIMPSON J.D., STELLO D., ZUCKER D.B., ZWITTER T., BEESON K.L., BUCK T., CASAGRANDE L., CLARK J.T., COTAR K., DA COSTA G.S., DE GRIJS R., FEUILLET D., HORNER J., KAFLE P.R., KHANNA S., KOBAYASHI C., LIU F., MONTET B.T., NANDAKUMAR G., NATAF D.M., NESS M.K., SPINA L., TEPPER-GARCIA T., TING Y.-S., TRAVEN G., VOGRINCIC R., WITTENMYER R.A., WYSE R.F.G., ZERJAL M., (The GALAH Collaboration)
	Mon. Not. R. Astron. Soc., 506, 150-201 (2021)
	The GALAH+ survey: Third data release.
o	<GALAH NNNNNNNNNNNNNNN> N=588571.
=E=	Catalogue in electronic form as <J/ApJS/228/24/>
=E=	Catalogue in electronic form as <J/MNRAS/465/3203/>
=E=	Catalogue in electronic form as <J/MNRAS/478/4513/>
=E=	Catalogue in electronic form as <J/MNRAS/506/150/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GALEX
GALEX	(Galaxy Evolution Explorer)
*****	Avoid the usage of GALEX, prefer [AIC2005]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GALEX
GALEX	(Galaxy Evolution Explorer)
*****	Avoid the usage of GALEX, prefer [CBH2010]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GALEX
GALEX	(Galaxy Evolution Explorer)
*****	Avoid the usage of GALEX, prefer [FPK2009]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GALEX
GALEX	(Galaxy Evolution Explorer)
Write:	<<GALEX NNNNNNNNNNNNNNNNNNN>> <<GALEX JHHMMSS.s+DDMMSS>>
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Note:	All GALEX data is made publically available through MAST (STScI archive) in yearly General Releases (GR) and also in smaller incremental releases to the archive every (approximetly) 4 months. The last data release is GR6/7. To access GALEX data, and for more information, visit http://galex.stsci.edu
Notes:	Longer formats (JHHMMSS.ss+DDMMSS.s, JHHMMSS.ss+DDMMSS.ss) are also found in the literature. They may be truncated in SIMBAD. As of May 2023, the format 'NNNNNNNNNNNNNNNNNNN' is not used in SIMBAD.
=E=	Catalogue in electronic form as II/312
=E=	Catalogue in electronic form as II/335
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GALEX
GALEX	(Galaxy Evolution Explorer)
Write:	<<GALEX NNNNNNNNNNNNNNNNNNN>> <<GALEX JHHMMSS.s+DDMMSS>>
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Note:	All GALEX data is made publically available through MAST (STScI archive) in yearly General Releases (GR) and also in smaller incremental releases to the archive every (approximetly) 4 months. The last data release is GR6/7. To access GALEX data, and for more information, visit http://galex.stsci.edu
Notes:	Longer formats (JHHMMSS.ss+DDMMSS.s, JHHMMSS.ss+DDMMSS.ss) are also found in the literature. They may be truncated in SIMBAD. As of May 2023, the format 'NNNNNNNNNNNNNNNNNNN' is not used in SIMBAD.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GALEX
GALEX	(Galaxy Evolution Explorer)
*****	Avoid the usage of GALEX, prefer [GBM2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GALEX
GALEX	(Galaxy Evolution Explorer)
*****	Avoid the usage of GALEX, prefer [VKN2010]
Origin	of the Acronym: L (2010MNRAS.404L..40V)
Details on Acronym: GALEXASC
GALEXASC	(GALEX All-Sky Survey Source Catalog)
Write:	<<GALEXASC JHHMMSS.ss+DDMMSS.s>>
N:	about 40 millions
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Note:	Covering a total of 26300 sq. deg. of sky, the GALEX All-Sky Survey Source Catalog consists of all GALEX observations with exposure times below 800s and reaches a depth of NUV 21 (AB mag). For more information, visit: https://archive.stsci.edu/prepds/gcat/ See also GALEXMSC, GALEXKEP.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GALEXKEP
GALEXKEP	(GALEX source catalog in the KEPler field) (Not yet in Simbad)
Write:	<<GALEXKEP JHHMMSS.ss+DDMMSS.s>>
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Note:	The GALEX Source Catalog in the Kepler Field (Kepler GCAT) is very similar to the GALEX All-Sky Survey Source Catalog and the GALEX Medium Imaging Survey Catalog. It includes data up through GR7, but only for the area of sky within and near the Kepler field. For more information, visit: https://archive.stsci.edu/prepds/gcat/ See also GALEXASC, GALEXMSC.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GALEXMSC
GALEXMSC	(GALEX Medium Imaging Survey Catalog)
Write:	<<GALEXMSC JHHMMSS.ss+DDMMSS.s>>
N:	about 22 millions
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Note:	The GALEX Medium Imaging Survey Catalog covers a region of 5000 sq. deg. of sky, with exposure times between 800s and 10000s and reaches a depth of NUV 23 (AB mag). For more information, visit: https://archive.stsci.edu/prepds/gcat/ See also GALEXASC, GALEXKEP.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Gallais
Gallais	(Gallais)
*****	Avoid the usage of Gallais, prefer [GRL91]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GAM2001a]
[GAM2001a]	(Garcia-Lorenzo+Arribas+Mediavilla+, 2001) (Not yet in Simbad)
Write:	<<[GAM2001a] A>>
N:	7
Object:	Component (SIMBAD class: PartofG = Part of a Galaxy)
Note:	N=7 distinct components or regions of ionized gas in NGC 2992.
in source:	NGC 2992
Ref:	=2001A&A...378..787G
by	GARCIA-LORENZO B. , ARRIBAS S., MEDIAVILLA E.
	Astron. Astrophys., 378, 787-799 (2001)
	Stellar and ionized gas kinematics of the interacting Seyfert 1.9 galaxy NGC 2992.
o	Table 1: <[GAM200a] A> (Nos A-G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GAM2001b]
[GAM2001b]	(Goudfrooij+Alonso+Maraston+, 2001) (Not yet in Simbad)
Write:	<<[GAM2001b] WFPC2 +xx.xx+yy.yy>> <<[GAM2001b] ESO-NTT +xxx.xx+yyy.yy>>
N:	50+50
Object:	Poss. GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	See also [GMK2001].
in source:	NGC 1316
Ref:	=2001MNRAS.328..237G
by	GOUDFROOIJ P. , ALONSO M.V., MARASTON C., MINNITI D.
	Mon. Not. R. Astron. Soc., 328, 237-256 (2001)
	The star cluster system of the 3-Gyr-old merger remnant NGC 1316: clues from optical and near-infrared photometry.
o	Table A1: <[GAM2001b] WFPC2 +xx.xx+yy.yy> N=50. Table A2: <[GAM2001b] ESO-NTT +xxx.xx+yyy.yy> N=50.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GAMA
GAMA	(Galaxy And Mass Assembly)
Write:	<<GAMA JHHMMSS.ss+DDMMSS.s>>
N:	265958
Object:	G (SIMBAD class: Galaxy)
Note:	GAMA is the Galaxy And Mass Assembly Survey (http://www.gama-survey.org/ and also http://star-www.st-and.ac.uk/gama/ ) which is a galaxy redshift and multiwavelength photometric survey using spectra from the AAT and photometry from SDSS, UKIDSS, VISTA-VIKING, VST-KIDSS, GALEX, Herschel ATLAS, and many other surveys, to construct a premier galaxy database. The GAMA first public data release occurs on 25 June 2010. The GAMA survey extends across three equatorial regions (G09, G12, and G15), and two southern regions (G02 and G23). 2011MNRAS.413..971D: DR1 (N=114441) - regions G09, G12, G15. 2015MNRAS.452.2087L: DR2 (N=72225) - regions G09, G12, G15. 2018MNRAS.474.3875B: DR3 (N=215260) - regions G02, G09, G12, G15. 2022MNRAS.513..439D: Unlike previous data releases, DR4 is not a static data release - regions G02, G09, G12, G15, G23.
Ref:	=2011MNRAS.413..971D
by	DRIVER S.P. , HILL D.T., KELVIN L.S., ROBOTHAM A.S.G., LISKE J., NORBERG P., BALDRY I.K., BAMFORD S.P., HOPKINS A.M., LOVEDAY J., PEACOCK J.A., ANDRAE E., BLAND-HAWTHORN J., BROUGH S., BROWN M.J.I., CAMERON E., CHING J.H.Y., COLLESS M., CONSELICE C.J., CROOM S.M., CROSS N.J.G., DE PROPRIS R., DYE S., DRINKWATER M.J., ELLIS S., GRAHAM A.W., GROOTES M.W., GUNAWARDHANA M., JONES D.H., VAN KAMPEN E., MARASTON C., NICHOL R.C., PARKINSON H.R., PHILLIPPS S., PIMBBLET K., POPESCU C.C., PRESCOTT M., ROSEBOOM I.G., SADLER E.M., SANSOM A.E., SHARP R.G., SMITH D.J.B., TAYLOR E., THOMAS D., TUFFS R.J., WIJESINGHE D., DUNNE L., FRENK C.S., JARVIS M.J., MADORE B.F., MEYER M.J., SEIBERT M., STAVELEY-SMITH L., SUTHERLAND W.J., WARREN S.J.
	Mon. Not. R. Astron. Soc., 413, 971-995 (2011)
	Galaxy and mass assembly (GAMA): survey diagnostics and core data release.
o	gamacore.dat: <GAMA JHHMMSS.ss+DDMMSS.s> = <GAMA NNNNNN> N=114441 among (Nos 6802-751324).
Ref:	=2015MNRAS.452.2087L
by	LISKE J. , BALDRY I.K., DRIVER S.P., TUFFS R.J., ALPASLAN M., ANDRAE E., BROUGH S., CLUVER M.E., GROOTES M.W., GUNAWARDHANA M.L.P., KELVIN L.S., LOVEDAY J., ROBOTHAM A.S.G., TAYLOR E.N., BAMFORD S.P., BLAND-HAWTHORN J., BROWN M.J.I., DRINKWATER M., HOPKINS A.M., MEYER M.J., NORBERG P., PEACOCK J.A., AGIUS N.K., ANDREWS S.K., BAUER A.E., CHING J.H.Y., COLLESS M., CONSELICE C.J., CROOM S.M., DAVIES L.J.M., DE PROPRIS R., DUNNE L., EARDLEY E.M., ELLIS S., FOSTER C., FRENK C.S., HAUSSLER B., HOLWERDA B.W., HOWLETT C., IBARRA H., JARVIS M.J., JONES D.H., KAFLE P.R., LACEY C.G., LANGE R., LARA-LOPEZ M.A., LOPEZ-SANCHEZ A.R., MADDOX S., MADORE B.F., McNAUGHT-ROBERTS T., MOFFETT A.J., NICHOL R.C., OWERS M.S., PALAMARA D., PENNY S.J., PHILLIPPS S., PIMBBLET K.A., POPESCU C.C., PRESCOTT M., PROCTOR R., SADLER E.M., SANSOM A.E., SEIBERT M., SHARP R., SUTHERLAND W., VAZQUEZ-MATA J.A., VAN KAMPEN E., WILKINS S.M., WILLIAMS R., WRIGHT A.H.
	Mon. Not. R. Astron. Soc., 452, 2087-2126 (2015)
	Galaxy And Mass Assembly (GAMA): end of survey report and data release 2.
o	inputcat.dat : <GAMA NNNNNN> (Nos 0-960509). tiling.dat: <GAMA NNNNNN> N=72225 among (Nos 6802-960508).
Ref:	=2018MNRAS.474.3875B
by	BALDRY I.K. , LISKE J., BROWN M.J.I., ROBOTHAM A.S.G., DRIVER S.P., DUNNE L., ALPASLAN M., BROUGH S., CLUVER M.E., EARDLEY E., FARROW D.J., HEYMANS C., HILDEBRANDT H., HOPKINS A.M., KELVIN L.S., LOVEDAY J., MOFFETT A.J., NORBERG P., OWERS M.S., TAYLOR E.N., WRIGHT A.H., BAMFORD S.P., BLAND-HAWTHORN J., BOURNE N., BREMER M.N., COLLESS M., CONSELICE C.J., CROOM S.M., DAVIES L.J.M., FOSTER C., GROOTES M.W., HOLWERDA B.W., JONES D.H., KAFLE P.R., KUIJKEN K., LARA-LOPEZ M.A., LOPEZ-SANCHEZ A.R., MEYER M.J., PHILLIPPS S., SUTHERLAND W.J., VAN KAMPEN E., WILKINS S.M.
	Mon. Not. R. Astron. Soc., 474, 3875-3888 (2018)
	Galaxy And Mass Assembly: the G02 field, Herschel-ATLAS target selection and data release 3.
o	<GAMA JHHMMSS.ss+DDMMSS.s> N=214624 = <GAMA NNNNNNN> N=214624.
Ref:	=2022MNRAS.513..439D
by	DRIVER S.P. , BELLSTEDT S., ROBOTHAM A.S.G., BALDRY I.K., DAVIES L.J., LISKE J., OBRESCHKOW D., TAYLOR E.N., WRIGHT A.H., ALPASLAN M., BAMFORD S.P., BAUER A.E., BLAND-HAWTHORN J., BILICKI M., BRAVO M., BROUGH S., CASURA S., CLUVER M.E., COLLESS M., CONSELICE C.J., CROOM S.M., DE JONG J., D'EUGENIO F., DE PROPRIS R., DOGRUEL B., DRINKWATER M.J., DVORNIK A., FARROW D.J., FRENK C.S., GIBLIN B., GRAHAM A.W., GROOTES M.W., GUNAWARDHANA M.L.P., HASHEMIZADEH A., HAUSSLER B., HEYMANS C., HILDEBRANDT H., HOLWERDA B.W., HOPKINS A.M., JARRETT T.H., HEATH JONES D., KELVIN L.S., KOUSHAN S., KUIJKEN K., LARA-LOPEZ M.A., LANGE R., LOPEZ-SANCHEZ A.R., LOVEDAY J., MAHAJAN S., MEYER M., MOFFETT A.J., NAPOLITANO N.R., NORBERG P., OWERS M.S., RADOVICH M., RAOUF M., PEACOCK J.A., PHILLIPPS S., PIMBBLET K.A., POPESCU C., SAID K., SANSOM A.E., SEIBERT M., SUTHERLAND W.J., THORNE J.E., TUFFS R.J., TURNER R., VAN DER WEL A., VAN KAMPEN E., WILKINS S.M.
	Mon. Not. R. Astron. Soc., 513, 439-467 (2022)
	Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions.
o	<GAMA JHHMMSS.ss+DDMMSS.s> N=265958 = <GAMA NNNNNNN> N=265958. Anglo-Australian Observatory
=E=	Catalogue in electronic form as J/MNRAS/413/971
=E=	Catalogue in electronic form as J/MNRAS/452/2087
=E=	Catalogue in electronic form as <J/MNRAS/474/3875/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: GAMA
GAMA	(Galaxy And Mass Assembly)
Write:	<<GAMA NNNNNNN>>
N:	265958
Object:	G (SIMBAD class: Galaxy)
Note:	GAMA is the Galaxy And Mass Assembly Survey (http://www.gama-survey.org/ and also http://star-www.st-and.ac.uk/gama/ ) which is a galaxy redshift and multiwavelength photometric survey using spectra from the AAT and photometry from SDSS, UKIDSS, VISTA-VIKING, VST-KIDSS, GALEX, Herschel ATLAS, and many other surveys, to construct a premier galaxy database. The GAMA first public data release occurs on 25 June 2010. The GAMA survey extends across three equatorial regions (G09, G12, and G15), and two southern regions (G02 and G23). 2011MNRAS.413..971D: DR1 (N=114441) - regions G09, G12, G15. 2015MNRAS.452.2087L: DR2 (N=72225) - regions G09, G12, G15. 2018MNRAS.474.3875B: DR3 (N=215260) - regions G02, G09, G12, G15. 2022MNRAS.513..439D: Unlike previous data releases, DR4 is not a static data release - regions G02, G09, G12, G15, G23.
Ref:	=2011MNRAS.413..971D
by	DRIVER S.P. , HILL D.T., KELVIN L.S., ROBOTHAM A.S.G., LISKE J., NORBERG P., BALDRY I.K., BAMFORD S.P., HOPKINS A.M., LOVEDAY J., PEACOCK J.A., ANDRAE E., BLAND-HAWTHORN J., BROUGH S., BROWN M.J.I., CAMERON E., CHING J.H.Y., COLLESS M., CONSELICE C.J., CROOM S.M., CROSS N.J.G., DE PROPRIS R., DYE S., DRINKWATER M.J., ELLIS S., GRAHAM A.W., GROOTES M.W., GUNAWARDHANA M., JONES D.H., VAN KAMPEN E., MARASTON C., NICHOL R.C., PARKINSON H.R., PHILLIPPS S., PIMBBLET K., POPESCU C.C., PRESCOTT M., ROSEBOOM I.G., SADLER E.M., SANSOM A.E., SHARP R.G., SMITH D.J.B., TAYLOR E., THOMAS D., TUFFS R.J., WIJESINGHE D., DUNNE L., FRENK C.S., JARVIS M.J., MADORE B.F., MEYER M.J., SEIBERT M., STAVELEY-SMITH L., SUTHERLAND W.J., WARREN S.J.
	Mon. Not. R. Astron. Soc., 413, 971-995 (2011)
	Galaxy and mass assembly (GAMA): survey diagnostics and core data release.
o	gamacore.dat: <GAMA JHHMMSS.ss+DDMMSS.s> = <GAMA NNNNNN> N=114441 among (Nos 6802-751324).
Ref:	=2015MNRAS.452.2087L
by	LISKE J. , BALDRY I.K., DRIVER S.P., TUFFS R.J., ALPASLAN M., ANDRAE E., BROUGH S., CLUVER M.E., GROOTES M.W., GUNAWARDHANA M.L.P., KELVIN L.S., LOVEDAY J., ROBOTHAM A.S.G., TAYLOR E.N., BAMFORD S.P., BLAND-HAWTHORN J., BROWN M.J.I., DRINKWATER M., HOPKINS A.M., MEYER M.J., NORBERG P., PEACOCK J.A., AGIUS N.K., ANDREWS S.K., BAUER A.E., CHING J.H.Y., COLLESS M., CONSELICE C.J., CROOM S.M., DAVIES L.J.M., DE PROPRIS R., DUNNE L., EARDLEY E.M., ELLIS S., FOSTER C., FRENK C.S., HAUSSLER B., HOLWERDA B.W., HOWLETT C., IBARRA H., JARVIS M.J., JONES D.H., KAFLE P.R., LACEY C.G., LANGE R., LARA-LOPEZ M.A., LOPEZ-SANCHEZ A.R., MADDOX S., MADORE B.F., McNAUGHT-ROBERTS T., MOFFETT A.J., NICHOL R.C., OWERS M.S., PALAMARA D., PENNY S.J., PHILLIPPS S., PIMBBLET K.A., POPESCU C.C., PRESCOTT M., PROCTOR R., SADLER E.M., SANSOM A.E., SEIBERT M., SHARP R., SUTHERLAND W., VAZQUEZ-MATA J.A., VAN KAMPEN E., WILKINS S.M., WILLIAMS R., WRIGHT A.H.
	Mon. Not. R. Astron. Soc., 452, 2087-2126 (2015)
	Galaxy And Mass Assembly (GAMA): end of survey report and data release 2.
o	inputcat.dat : <GAMA NNNNNN> (Nos 0-960509). tiling.dat: <GAMA NNNNNN> N=72225 among (Nos 6802-960508).
Ref:	=2018MNRAS.474.3875B
by	BALDRY I.K. , LISKE J., BROWN M.J.I., ROBOTHAM A.S.G., DRIVER S.P., DUNNE L., ALPASLAN M., BROUGH S., CLUVER M.E., EARDLEY E., FARROW D.J., HEYMANS C., HILDEBRANDT H., HOPKINS A.M., KELVIN L.S., LOVEDAY J., MOFFETT A.J., NORBERG P., OWERS M.S., TAYLOR E.N., WRIGHT A.H., BAMFORD S.P., BLAND-HAWTHORN J., BOURNE N., BREMER M.N., COLLESS M., CONSELICE C.J., CROOM S.M., DAVIES L.J.M., FOSTER C., GROOTES M.W., HOLWERDA B.W., JONES D.H., KAFLE P.R., KUIJKEN K., LARA-LOPEZ M.A., LOPEZ-SANCHEZ A.R., MEYER M.J., PHILLIPPS S., SUTHERLAND W.J., VAN KAMPEN E., WILKINS S.M.
	Mon. Not. R. Astron. Soc., 474, 3875-3888 (2018)
	Galaxy And Mass Assembly: the G02 field, Herschel-ATLAS target selection and data release 3.
o	<GAMA JHHMMSS.ss+DDMMSS.s> N=214624 = <GAMA NNNNNNN> N=214624.
Ref:	=2022MNRAS.513..439D
by	DRIVER S.P. , BELLSTEDT S., ROBOTHAM A.S.G., BALDRY I.K., DAVIES L.J., LISKE J., OBRESCHKOW D., TAYLOR E.N., WRIGHT A.H., ALPASLAN M., BAMFORD S.P., BAUER A.E., BLAND-HAWTHORN J., BILICKI M., BRAVO M., BROUGH S., CASURA S., CLUVER M.E., COLLESS M., CONSELICE C.J., CROOM S.M., DE JONG J., D'EUGENIO F., DE PROPRIS R., DOGRUEL B., DRINKWATER M.J., DVORNIK A., FARROW D.J., FRENK C.S., GIBLIN B., GRAHAM A.W., GROOTES M.W., GUNAWARDHANA M.L.P., HASHEMIZADEH A., HAUSSLER B., HEYMANS C., HILDEBRANDT H., HOLWERDA B.W., HOPKINS A.M., JARRETT T.H., HEATH JONES D., KELVIN L.S., KOUSHAN S., KUIJKEN K., LARA-LOPEZ M.A., LANGE R., LOPEZ-SANCHEZ A.R., LOVEDAY J., MAHAJAN S., MEYER M., MOFFETT A.J., NAPOLITANO N.R., NORBERG P., OWERS M.S., RADOVICH M., RAOUF M., PEACOCK J.A., PHILLIPPS S., PIMBBLET K.A., POPESCU C., SAID K., SANSOM A.E., SEIBERT M., SUTHERLAND W.J., THORNE J.E., TUFFS R.J., TURNER R., VAN DER WEL A., VAN KAMPEN E., WILKINS S.M.
	Mon. Not. R. Astron. Soc., 513, 439-467 (2022)
	Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions.
o	<GAMA JHHMMSS.ss+DDMMSS.s> N=265958 = <GAMA NNNNNNN> N=265958.
=E=	Catalogue in electronic form as J/MNRAS/413/971
=E=	Catalogue in electronic form as J/MNRAS/452/2087
=E=	Catalogue in electronic form as <J/MNRAS/474/3875/>
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GAN2001]
[GAN2001]	(Grosso+Alves+Neuhauser+, 2001)
Write:	<<[GAN2001] AN>>
N:	17
Object:	H-alpha Knot (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	H2 knots produced by shocks on the H2 map of the rho Oph Cloud.
in source:	NAME rho Oph Cloud
Ref:	=2001A&A...380L...1G
by	GROSSO N. , ALVES J., NEUHAEUSER R., MONTMERLE T.
	Astron. Astrophys., 380, 1-4 (2001)
	Discovery of new embedded Herbig-Haro objects in the ρ Ophiuchi dark cloud.
o	Table 1, Fig.2c: <[GAN2001] AN> (Nos A1-A5, B1-B7, C1-C5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GAP2005]
[GAP2005]	(Galliano+Alloin+Pantin+, 2005)
Write:	<<[GAP2005] NGC NNNN MN>> <<[GAP2005] Circinus MN>> <<[GAP2005] I Zw 1 MN>> <<[GAP2005] II Zw 136 MN>>
N:	28
Object:	(Mid IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	ESO 3.6m telescope TIMMI2 Mid-IR observations of active galaxies.
in source:	NGC 253
in source:	NAME Circinus Galaxy
in source:	NGC 1808
in source:	NGC 1365
in source:	NGC 2992
in source:	NGC 5995
in source:	ZW I 1
in source:	ZW II 136
Ref:	=2005A&A...438..803G
by	GALLIANO E. , ALLOIN D., PANTIN E., LAGAGE P.O., MARCO O.
	Astron. Astrophys., 438, 803-820 (2005)
	Mid-infrared imaging of active galaxies. Active nuclei and embedded star clusters.
o	In table 1 coordinates of NGC 2992 correspond to another object (UGC 11763).
o	Fig.2, Table 2: <[GAP2005] NGC NNNN MN>, <[GAP2005] Circinus MN>, <[GAP2005] I Zw 1 MN>, <[GAP2005] II Zw 136 MN>, N=6+1+9+6+1+1+1+1.
Ref:	=2007ApJ...654..782S
by	SAKAMOTO K. , HO P.T.P., MAO R.-Q., MATSUSHITA S., PECK A.B.
	Astrophys. J., 654, 782-798 (2007)
	Detection of CO hot spots associated with young clusters in the southern starburst galaxy NGC 1365.
o	Table 4, Fig.9: <[GAP2005] NGC 1365 MN> (Nos M7, M8) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GAP2008]
[GAP2008]	(Galliano+Alloin+Pantin+, 2008) (Not yet in Simbad)
Write:	<<[GAP2008] CN>>
N:	3
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	VLT ISAAC and VISIR maps in NGC 1365. N=3 sources identified as star clusters.
in source:	NGC 1365
Ref:	=2008A&A...492....3G
by	GALLIANO E. , ALLOIN D., PANTIN E., GRANATO G.L., DELVA P., SILVA L., LAGAGE P.O., PANUZZO P.
	Astron. Astrophys., 492, 3-22 (2008)
	Extremely massive young clusters in NGC1365.
o	Figs 2,3, Table 1: <[GAP2008] CN> (Nos C1-C3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GAP2015]
[GAP2015]	(Garcia-Gonzalez+Alonso-Herrero+Perez-Gonzalez+, 2015)
Write:	<<[GAP2015] NNNNN>>
N:	39+55
Object:	AGN (SIMBAD class: AGN = Active Galaxy Nucleus)
Note:	Spitzer MIPS 24µm identification of N=94 AGN through mid-IR variability in the GOODS-South field.
in source:	NAME GOODS Southern Field
Ref:	=2015MNRAS.446.3199G
by	GARCIA-GONZALEZ J. , ALONSO-HERRERO A., PEREZ-GONZALEZ P.G., HERNAN-CABALLERO A., SARAJEDINI V.L., VILLAR V.
	Mon. Not. R. Astron. Soc., 446, 3199-3223 (2015)
	Selection of AGN candidates in the GOODS-South Field through Spitzer/MIPS 24 µm variability.
o	Tables D1, E1: <[GAP2015] NNNNN> N=39+55 among (Nos 13-16416).
=E=	Catalogue in electronic form as J/MNRAS/446/3199
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Gapo
Gapo	(Gaposchkin)
Write:	<<Gapo NNNa>>
N:	226
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	(Nos 1-223), field II in M 31. Fields in I, III and IV in M 31: see BASW and [BS63]
in source:	M 31 = NGC 224
Ref:	=1962AJ.....67..334G
by	GAPOSCHKIN S.
	Astron. J., 67, 334-357 (1962)
	223 Variables in the Andromeda Nebula.
o	Table II: <GAPO NNNa> (Nos 1-223, 39a, 57a, 75a, Nos 214, 218 missing) N=225.
Details on Acronym: GAS
GAS	(Goods Area South)
*****	Avoid the usage of GAS, prefer [RPF2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GASS
GASS	(GALEX Arecibo SDSS Survey)
Write:	<<GASS NNNNNN>>
N:	176+240+250+532+208
Object:	G (SIMBAD class: Galaxy)
Note:	Arecibo HI spectroscopy of a sample of about 1000 galaxies selected from the SDSS spectroscopic and GALEX imaging surveys. 2010MNRAS.403..683C: GASS DR1 (N=176) 2012A&A...544A..65C: GASS DR2 (N=240) 2013MNRAS.436...34C: GASS DR3 (final data release, N=250) For more information on the GASS survey, visit https://wwwmpa.mpa-garching.mpg.de/GASS/index.php The low-mass extension of GASS (hereafter GASS-low) includes new Arecibo observations for N=208 galaxies. This program is described in Catinella et al. 2018MNRAS.476..875C. The combination of GASS and GASS-low is referred to as the extended GASS (xGASS) survey and results in a representative sample of 1179 galaxies covering the 9<log M_/M_☉<11.5 stellar interval. More information is available on the website: http://xgass.icrar.org/ The COLD GASS* (CO Legacy Database for GASS) is a large program that measured the molecular gas contents of 366 massive galaxies through IRAM 30-m CO(1-0) observations. The program is described in Saintonge et al. 2011MNRAS.415...32S. More information is available on the website: http://www.mpa-garching.mpg.de/COLD_GASS/data.shtml The initial COLD GASS survey targeted 366 galaxies with M_>10¹⁰M_☉ and 0.025<z<0.050. It was followed by a second effort, to extend the sample in the stellar mass range of 10⁹<M_/M_☉<10¹⁰: this second survey (166 galaxies) is referred to as COLD GASS-low. Galaxies with six-digit IDs are part of COLD GASS-low. The combined xCOLD GASS (extended COLD GASS) sample therefore contains 532 galaxies with IRAM 30 m CO(1-0) observations and is described in 2017ApJS..233...22S. For more information, visit: http://www.star.ucl.ac.uk/xCOLDGASS/
Ref:	=2010MNRAS.403..683C
by	CATINELLA B. , SCHIMINOVICH D., KAUFFMANN G., FABELLO S., WANG J., HUMMELS C., LEMONIAS J., MORAN S.M., WU R., GIOVANELLI R., HAYNES M.P., HECKMAN T.M., BASU-ZYCH A.R., BLANTON M.R., BRINCHMANN J., BUDAVARI T., GONCALVES T., JOHNSON B.D., KENNICUTT R.C., MADORE B.F., MARTIN C.D., RICH M.R., TACCONI L.J., THILKER D.A., WILD V., WYDER T.K.
	Mon. Not. R. Astron. Soc., 403, 683-708 (2010)
	The GALEX Arecibo SDSS survey - I. Gas fraction scaling relations of massive galaxies and first data release.
o	Tables 1-3: <GASS NNNNN> N=176 among (Nos 3261-57017).
Ref:	=2012A&A...544A..65C
by	CATINELLA B. , SCHIMINOVICH D., KAUFFMANN G., FABELLO S., HUMMELS C., LEMONIAS J., MORAN S.M., WU R., COOPER A., WANG J.
	Astron. Astrophys., 544A, 65-65 (2012)
	The GALEX Arecibo SDSS survey. VI. Second data release and updated gas fraction scaling relations.
o	<GASS NNNNN> N=240 among (Nos 3151-57099).
Ref:	=2013MNRAS.436...34C
by	CATINELLA B. , SCHIMINOVICH D., CORTESE L., FABELLO S., HUMMELS C.B., MORAN S.M., LEMONIAS J.J., COOPER A.P., WU R., HECKMAN T.M., WANG J.
	Mon. Not. R. Astron. Soc., 436, 34-70 (2013)
	The GALEX Arecibo SDSS survey - VIII. Final data release. The effect of group environment on the gas content of massive galaxies.
o	<GASS NNNNN> N=250 among (Nos 3157-56662).
Ref:	=2017ApJS..233...22S
by	SAINTONGE A. , CATINELLA B., TACCONI L.J., KAUFFMANN G., GENZEL R., CORTESE L., DAVE R., FLETCHER T.J., GRACIA-CARPIO J., KRAMER C., HECKMAN T.M., JANOWIECKI S., LUTZ K., ROSARIO D., SCHIMINOVICH D., SCHUSTER K., WANG J., WUYTS S., BORTHAKUR S., LAMPERTI I., ROBERTS-BORSANI G.W.
	Astrophys. J., Suppl. Ser., 233, 22-22 (2017)
	xCOLD GASS: the complete IRAM 30 m legacy survey of molecular gas for galaxy evolution studies.
o	<GASS NNNNNN> N=366+166 among (Nos 522-57017, 101000-124028).
Ref:	=2018MNRAS.476..875C
by	CATINELLA B. , SAINTONGE A., JANOWIECKI S., CORTESE L., DAVE R., LEMONIAS J.J., COOPER A.P., SCHIMINOVICH D., HUMMELS C.B., FABELLO S., GEREB K., KILBORN V., WANG J.
	Mon. Not. R. Astron. Soc., 476, 875-895 (2018)
	xGASS: total cold gas scaling relations and molecular-to-atomic gas ratios of galaxies in the local Universe.
o	Table A1: <GASS NNNNNN> N=208 among (Nos 101000-124012).
=E=	Catalogue in electronic form as <J/MNRAS/403/683/>
=E=	Catalogue in electronic form as <J/MNRAS/415/32/>
=E=	Catalogue in electronic form as <J/A+A/544/A65/>
=E=	Catalogue in electronic form as <J/MNRAS/436/34/>
=E=	Catalogue in electronic form as <J/ApJS/233/22/>
=E=	Catalogue in electronic form as <J/MNRAS/476/875/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Gat
Gat	(Gatewood+)= AO
Write:	<<GAT NNNN>>
N:	1387
Object:	* (SIMBAD class: Star)
Ref:	=1973AJ.....78..769G
by	GATEWOOD G. , EICHHORN H.
	Astron. J., 78, 769-776 (1973)
	An unsuccessful search for a planetary companion of Barnard's star (BD +4 3561).
o	<GAT NN> (Nos 1-22)
Ref:	=1974ApJ...194..637B
by	BEARDSLEY W.R. , GATEWOOD G., KAMPER K.W.
	Astrophys. J., 194, 637-643 (1974)
	A study of an early flare, radial velocities, and parallax residuals for possible orbital motion of HD 103095 (Groombridge 1830).
o	<GAT NN> (Nos 23-36)
Ref:	=1974AJ.....79...52G
by	GATEWOOD G.
	Astron. J., 79, 52-53 (1974)
	An astrometric study of Lalande 21185.
o	<GAT NN> (Nos 52-69)
Ref:	=1974PASP...86..448B
by	BREAKIRON L.A. , GATEWOOD G.
	Publ. Astron. Soc. Pac., 86, 448-454 (1974)
	An astrometric study of the spectroscopic binary χ Draconis.
o	<GAT NNN> (Nos 94-120)
Ref:	=1974AJ.....79..815G
by	GATEWOOD G. , RUSSEL J.
	Astron. J., 79, 815-818 (1974)
	Astrometric determination of the gravitational redshift of van Maanen 2 (EG 5).
o	<GAT NNN> (Nos 121-144)
Ref:	=1975AJ.....80..318B
by	BREAKIRON L.A. , GATEWOOD G.
	Astron. J., 80, 318-320 (1975)
	Parallax, mass, orbit of the 9 Puppis binary system.
o	<GAT NNN> (Nos 178-202).
Ref:	=1975AJ.....80..652R
by	RUSSELL J. , GATEWOOD G.
	Astron. J., 80, 652-654 (1975)
	Astrometric studies of the regions BD +17 4946, BD -5 3071, Ross 730-1.
o	<GAT NNN> (Nos 36-51), (Nos 82-93), (Nos 145-162).
Ref:	=1975AJ.....80..714B
by	BREAKIRON L.A. , DABROWSKI J.P., GATEWOOD G.
	Astron. J., 80, 714-718 (1975)
	Parallaxes, masses, and orbits of visual binaries η Coronae Borealis and Kuiper 37 (10 Ursae Majoris).
o	<GAT NNN> (Nos 163-177).
Ref:	=1975AJ.....80.1065G
by	GATEWOOD G. , BEHALL A.L.
	Astron. J., 80, 1065-1070 (1975)
	On the nature of the triple-star system 13 Ceti.
o	<GAT NN> (Nos 70-81).
Ref:	=1976ApJ...204L..89G
by	GATEWOOD G. , SOFIA S.
	Astrophys. J., 204, 89-90 (1976)
	The positions and proper motions of HZ Herculis and 12 neighboring stars.
o	<GAT NNN> (Nos 218-230)
Ref:	=1976AJ.....81..545R
by	RUSSELL J. , GATEWOOD G., STEIN J.W.
	Astron. J., 81, 545-547 (1976)
	Astrometric constants for SIGMA 282, BD +75 325, +66 550, Ross 142, and selected stars in those regions.
o	<GAT NNN> (Nos 231-292)
Ref:	=1976ApJ...209..525M
by	MARGON B. , LIEBERT J., GATEWOOD G., LAMPTON M., SPINRAD H., BOWYER S.
	Astrophys. J., 209, 525-535 (1976)
	An extrasolar extreme-ultraviolet object. II. The nature of HZ 43.
o	<GAT NNN> (Nos 293-305)
Ref:	=1977AJ.....82..364S
by	STEIN J.W. , DABROWSKI J.P., GATEWOOD G.
	Astron. J., 82, 364-367 (1977)
	Astrometric investigations of 91 and 92 Tauri, Lalande 20111, 18 Bootis, HD 187399 and selected field stars.
o	<GAT NNN> (Nos 306-363)
Ref:	=1978ApJ...225..191G
by	GATEWOOD G.D. , GATEWOOD C.V.
	Astrophys. J., 225, 191-197 (1978)
	A study of Sirius.
o	<GAT NNN> (Nos 458-484)
Ref:	=1978AJ.....83.1455R
by	RUSSELL J.L. , GATEWOOD G.D., WAGMAN N.E.
	Astron. J., 83, 1455-1458 (1978)
	Altair.
o	<GAT NNN> (Nos 538-564)
Ref:	=1980AJ.....85.1270R
by	RUSSELL J. , GATEWOOD G.
	Astron. J., 85, 1270-1273 (1980)
	The triple system Gliese 815 (Furuhjelm 54): an astrometric study.
o	<GAT NNN> (Nos 565-597)
Ref:	=1988ApJ...332..917G
by	GATEWOOD G. , DE JONGE J.K., CASTELAZ M., HAN I., PERSINGER T., PROSSER J., REILAND T., STEIN J.
	Astrophys. J., 332, 917-920 (1988)
	A study of Upgren 1.
o	error in table 1 GAT 695 is BD +37 2293 not 37 2296
o	<GAT NNN> (Nos 691-709)
Ref:	=1989AJ.....97.1189G
by	GATEWOOD G.
	Astron. J., 97, 1189-1196 (1989)
	Map determinations of the parallaxes of stars in the regions of HD 2665, BD +68 946, and λ Ophiuchi.
o	<GAT NNN> (Nos 710-747)
Ref:	=1989AJ.....97.1184C
by	CASTELAZ M.W.
	Astron. J., 97, 1184-1188 (1989)
	First detection of the astrometric orbit of the single-lined spectroscopic binary ε Librae.
o	<GAT NNN> (Nos 748-756)
Ref:	=1989AJ.....98.1768C
by	CASTELAZ M. , PERSINGER T.
	Astron. J., 98, 1768-1782 (1989)
	Spectral types and luminosity classifications of map region stars using UBVRI and DDO photometry.
o	misprint GAT 814=BD+56 2964 instead of GAT 809=BD+56 2964; GAT 792 is not BD+42 3333.
o	<GAT NNN> (Nos 757-815)
Ref:	=1990AJ....100.1621P
by	PERSINGER T. , CASTELAZ M.W.
	Astron. J., 100, 1621-1641 (1990)
	Spectroscopic parallaxes of map region stars from UBVRI, DDO, and uvbyH-β photometry.
o	<GAT NNN> (Nos 816-997)
Ref:	=1991AJ....102.2103C
by	CASTELAZ M.W. , PERSINGER T., STEIN J.W., PROSSER J., POWELL H.D.
	Astron. J., 102, 2103-2118 (1991)
	Photometry of astrometric reference stars.
o	Some positions listed in table 1 are not for equinox 2000.0 : stars around BD + 43 4305 and stars around Procyon.
o	<GAT NNNN> (Nos 1013-1215)
Ref:	=1992ApJ...392..710G
by	GATEWOOD G. , CASTELAZ M., DE JONGE J.K., PERSINGER T., STEIN J., STEPHENSON B.
	Astrophys. J., 392, 710-714 (1992)
	Map-based trigonometric parallaxes of open clusters. II. The Hyades: 51 Tauri.
o	<GAT NNN> (Nos 998-999).
Ref:	=1992PASP..104...23G
by	GATEWOOD G.
	Publ. Astron. Soc. Pac., 104, 23-28 (1992)
	An astrometric study of the mira variable R Leonis and the occultation binary 19 Leonis.
o	<GAT NNNN> No. 1000
Ref:	=1992AJ....104.1237G
by	GATEWOOD G. , STEIN J., KIEWIET DE JONGE J., PERSINGER T., REILAND B.
	Astron. J., 104, 1237-1247 (1992)
	Multichannel astrometric photometer and photographic astrometric studies in the regions of Lalande 21185, BD +56 2966, and HR 4784.
o	<GAT NNNN> (Nos 1001-1012), (Nos 1216-1254)
Ref:	=1993AJ....105.1179G
by	GATEWOOD G. , KIEWIET DE JONGE J., STEPHENSON B.
	Astron. J., 105, 1179-1187 (1993)
	Multi channel astrometric photometer parallax studies in the regions of Groombridge 1618, zet Bootis, sig Draconis.
o	<GAT NNNN> No. 1255
Ref:	=1993PASP..105.1101G
by	GATEWOOD G. , DE JONGE J.K., STEPHENSON B.
	Publ. Astron. Soc. Pac., 105, 1101-1106 (1993)
	One-milliarcsecond precision parallax studies in the regions of δ Cephei and EV Lacertae.
o	<GAT NNNN> (Nos 1256-1258)
Ref:	=1995AJ....109..434G
by	GATEWOOD G. , DE JONGE J.K., HEINTZ W.D.
	Astron. J., 109, 434-439 (1995)
	Astrometric studies in the region of Algol.
o	<GAT NNNN> (Nos 1262-1269)
Ref:	=1995ApJ...445..712G
by	GATEWOOD G.
	Astrophys. J., 445, 712-715 (1995)
	Map-based trigonometric parallaxes of open clusters : Coma.
o	<GAT NNNN> (Nos 1270-1271)
Ref:	=1995AJ....110.1860G
by	GATEWOOD G. , HAN I.
	Astron. J., 110, 1860-1865 (1995)
	A map based study of ADS 14893.
o	<GAT NNNN> (Nos 1286-1296)
Ref:	=2000ApJ...533..938G
by	GATEWOOD G. , DE JONGE J.K., HAN I.
	Astrophys. J., 533, 938-943 (2000)
	The Pleiades, map-based trigonometric parallaxes of open clusters. V.
o	T. 3 : misprints : GAT 826 = BD +23 515, GAT 827 = BD +24 556
o	Table 1: <GAT NNNN> (Nos 1297-1300).
Ref:	=2002PASP..114..224H
by	HAN I. , GATEWOOD G.
	Publ. Astron. Soc. Pac., 114, 224-228 (2002)
	A precise orbit determination of χ^{1} Orionis from astrometric and radial velocity data.
o	Table 1: <Gat NNN> (No. 1261) added.
Ref:	=2003AJ....125.1530G
by	GATEWOOD G. , COBAN L., HAN I.
	Astron. J., 125, 1530-1536 (2003)
	An astrometric study of the low-mass binary star Ross 614.
o	Tables 1, 2: <Gat NNNN> (Nos 1302-1312) added.
Ref:	=2005AJ....130..809G
by	GATEWOOD G.
	Astron. J., 130, 809-814 (2005)
	An astrometric study of the binary star α Ophiuchi.
o	Table 1: <Gat NNNN> (Nos 1313-1320, 1322-1323) added.
Ref:	=2008AJ....136..452G
by	GATEWOOD G.
	Astron. J., 136, 452-460 (2008)
	Astrometric studies of Aldebaran, Arcturus, Vega, the Hyades, and other regions.
o	Table 1: <Gat NNNN> N=26 among (Nos 1328-1366).
Ref:	=2009AJ....137..402G
by	GATEWOOD G. , COBAN L.
	Astron. J., 137, 402-405 (2009)
	Allegheny observatory parallaxes for late M dwarfs and white dwarfs.
o	In abstract LSPM 0607+7372 is a misprint for LSPM 0607+7332.
o	Table 1: <Gat NNNN> (Nos 1367-1387) added.
=E=	Catalogue in electronic form as <J/AJ/136/452/>
Details on Acronym: GAVC
GAVC	(GASS Anomalous Velocity Cloud)
Write:	<<GAVC GLLL.l+BB.b+VVV>>
N:	295
Object:	HVC (SIMBAD class: HVCld = High-velocity Cloud)
Note:	We are publishing a catalogue of high velocity clouds as discovered within the Galactic All Sky Survey (GASS) data. The catalogue paper is nearing submission and will contain a table of all HVCs found in GASS. We are submitting this application for a new acronym in order to facilitate reference to specific GASS HVCs in future follow-up work. The sensitivity of GASS to large scale structure as well as the way we identify HVCs using a floodfill sourcefinder makes a GHVC distinct from an HVC, in that our definition of a source may join several clouds that are connected at the 2 sigma level. Hence, we propose the new acronym GHVC to specifically designate a source as a GASS HVC, to make the origin of such a cloud clear. See GHVC. We have also added a further classification to the name: either GASS High Velocity Cloud (GHVC) or GASS Anomalous Velocity Cloud (GAVC). This is because the GAVCs do not meet the standard velocity criteria of an HVC, and are best classified as an anomalous velocity cloud pending further investigation into their physical properties. This is also made clear in the paper.
Ref:	=2013ApJS..209...12M
by	MOSS V.A. , McCLURE-GRIFFITHS N.M., MURPHY T., PISANO D.J., KUMMERFELD J.K., CURRAN J.R.
	Astrophys. J., Suppl. Ser., 209, 12 (2013)
	High-velocity clouds in the Galactic All Sky Survey. I. Catalog.
o	Table 1: <GHVC GLLL.l+BB.b+VVV> N=1693. Table 2: <GAVC GLLL.l+BB.b+VVV> N=295. University of Sydney/CSIRO Astronomy and Space Science
=E=	Catalogue in electronic form as J/ApJS/209/12
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: GB
GB	(Green Bank obs.)
*****	Avoid the usage of GB, prefer GB1
Details on Acronym: GB
GB	(Green Bank obs.)
*****	Avoid the usage of GB, prefer GB2
Details on Acronym: GB
GB	(Green Bank obs.)
*****	Avoid the usage of GB, prefer GB3
Details on Acronym: GB
GB	(Green Bank obs.)
*****	Avoid the usage of GB, prefer GB6
Details on Acronym: GB
GB	(Gamma Burst)
====>	Equivalent to: GRB
Origin	of the Acronym: L = Found in the literature
Details on Acronym: GB
GB	(Green Bank)
*****	Avoid the usage of GB, prefer [HMI96]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GB
GB	(G. Burbidge)
Write:	<<NAME GB N>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Ref:	=1967ApJ...150..783B
by	BURBIDGE E.M. , BURBIDGE G.R., SHELTON J.W.
	Astrophys. J., 150, 783-786 (1967)
	A peculiar galaxy that may be at a young evolutionary stage.
o	<NAME GB 1>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GB
GB	(Green Bank obs.)
*****	Avoid the usage of GB, prefer S3
Origin	of the Acronym: L = Found in the literature
Details on Acronym: GB07
GB07	(G. Battaglia, 2007)
Write:	<<GB07 TUCNNNN>> <<GB07 N3201-SNNN>> <<GB07 M68-SNNN>> <<GB07 M5-SNNNN>> <<GB07 SclNN>> <<GB07 FnxNN>>
N:	10+14+4+41+93+36
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT FLAMES observations of RGB stars in N=4 GCl and N=2 dwarf galaxies.
in source:	NGC 104 = 47 Tuc
in source:	NGC 3201
in source:	NGC 4590 = M 68
in source:	NGC 5904 = M 5
in source:	NAME Scl Dwarf Galaxy
in source:	NAME Fornax Dwarf Galaxy
Ref:	=2008MNRAS.383..183B
by	BATTAGLIA G. , IRWIN M., TOLSTOY E., HILL V., HELMI A., LETARTE B., JABLONKA P.
	Mon. Not. R. Astron. Soc., 383, 183-199 (2008)
	Analysis and calibration of CaII triplet spectroscopy of red giant branch stars from VLT/FLAMES observations.
o	Table 3: <GB07 TUCNNNN> N=10, <GB07 N3201-SNNN> N=14, <GB07 M68-SNNN> N=4, <GB07 M5-SNNNN> N=41. Table 4: <GB07 SclNN> (Nos Scl01 to Scl93), <GB07 FnxNN> (Nos Fnx01 to Fnx36).
=E=	Catalogue in electronic form as J/MNRAS/383/183
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GB1
GB1	(Green Bank obs., 1st survey)= (GB)
Write:	<<GB1 HHMM+DDdA>>
N:	1086
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Survey at 20cm.
Ref:	=1971A&A....14..215M
by	MASLOWSKI J.
	Astron. Astrophys., 14, 215-222 (1971)
	A Green Bank sky survey in search of radio sources at 1400 MHz. I. A spectral analysis of the 5C1 sources.
o	Table 1: <GB1 HHMM+DDd> N=32
Ref:	=1972A&A....16..197M
by	MASLOWSKI J.
	Astron. Astrophys., 16, 197-203 (1972)
	A Green Bank sky survey in search of radio sources at 1400 MHz. II. Spectral properties of the 5C1 and 5C2 sources.
o	Table 1: <GB1 HHMM+DDd> N=40
Ref:	=1972AcA....22..227M
by	MASLOWSKI J.
	Acta Astron., 22, 227-260 (1972)
	A Green Bank sky survey in search of radio sources at 1400 MHz. III. Positions and flux densities of the GB radio sources.
o	Table 1: <GB1 HHMM+DDdA> N=1086
=E=	Catalogue in electronic form as VIII/53
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GB2
GB2	(Green Bank obs., 2nd survey)= (GB)
Write:	<<GB2 HHMM+DDdA>>
N:	2084
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	The Green Banks catalogues are revised in 1998A&AS..128..153M, and 21 objects are added individually as GB/GB2 in some refs. Survey at 20cm.
Ref:	=1978AcA....28..367M
by	MACHALSKI J.
	Acta Astron., 28, 367-440 (1978)
	The Green Bank second survey of extragalactic radio sources at 1400 MHz. The catalogue of sources.
o	<GB2 HHMM+DDdA> N=2022
=E=	Catalogue in electronic form as J/A+AS/128/153
=E=	Catalogue in electronic form as VIII/53
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GB2001]
[GB2001]	(Genova+Beckman, 2001)= (AG)
Write:	<<[GB2001] AG N>>
N:	8
Object:	Interstellar Cloud (SIMBAD class: Cloud)
Note:	N=8 interstellar clouds in the second galactic quadrant, in the direction of the galactic Anticenter.
Ref:	=2001Ap&SS.276..187G
by	GENOVA R. , BECKMAN J.E.
	Astrophys. Space Sci., 276, 187-195 (2001)
	The local interstellar medium in the direction of the Galactic Anticentre.
o	Table 1: <[GB2001] AG N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GB2004]
[GB2004]	(Georgiev+Bomans, 2004)
Write:	<<[GB2004] DN>>
N:	8
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Rozhen National Astronomical Observatory observations of Holmberg IX. N=8 new Diffuse objects (letter 'D' in the format) are found.
in source:	Holmberg IX
Ref:	=2004A&A...423...87G
by	GEORGIEV T.B. , BOMANS D.J.
	Astron. Astrophys., 423, 87-95 (2004)
	BVR photometry of the resolved dwarf galaxy HoIX.
o	Table 1: <[GB2004] AN> (Nos D1-D8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GB3
GB3	(Green Bank obs., 3rd survey)= (GB)
Write:	<<GB3 HHMM+DDd>>
N:	502+174
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=502, GB3 radio-sources stronger than 112 mJy. Table 2: N=174, other sources reliably detected. Survey at 20cm.
Ref:	=1987AcA....37..163R
by	RYS S. , MACHALSKI J.
	Acta Astron., 37, 163-178 (1987)
	The Green Bank third (GB3) survey of extragalactic radiosources at 1400 MHz.
o	Tables 1, 2: <GB3 HHMM+DDd> N=502+174
=E=	Catalogue in electronic form as VIII/53
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GB6
GB6	(Green Bank obs., 6cm survey)= (GB)
Write:	<<GB6 BHHMM+DDMMa>> <<GB6 JHHMM+DDMMa>>
N:	75162
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Supersedses 87GB
Ref:	=1996ApJS..103..427G
by	GREGORY P.C. , SCOTT W.K., DOUGLAS K., CONDON J.J.
	Astrophys. J., Suppl. Ser., 103, 427-432 (1996)
	The GB6 catalog of radio sources.
o	Table 2: <GB6 BHHMM+DDMMa> = <GB6 JHHMM+DDMMa>, N=75162
=E=	Catalogue in electronic form as VIII/40
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 87GB
87GB	(1987, Green Bank obs.)
Write:	<<87GB HHMMSS.s+DDMMSS>>
N:	54579
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	The 91 m telescope in Green Bank was used during 1987 to map 6.0 sr of sky. N = 54579 discrete sources with angular sizes diameter < 10'.5 and stronger than S about 25 mJy derived from the maps
Ref:	=1991ApJS...75.1011G
by	GREGORY P.C. , CONDON J.J.
	Astrophys. J., Suppl. Ser., 75, 1011-1291 (1991)
	The 87GB catalog of radio sources covering 0° < del <+75° at 4.85 GHz.
o	Table 2: <87GB HHMMSS.s+DDMMSS> N=54579
=E=	Catalogue in electronic form as VIII/14
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GB97]
[GB97]	(Guillemin+Bergeron, 1997)
Write:	<<[GB97] HHMM+DDd GN>>
N:	41
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Tables 2, 3, 4, Figs 2, 3: The authors used no format for the different galaxies (except in Figs 2 and 3). We called them 'GN' in each of the 25 fields. See also [B86b], [BB86b], [BDK87], [B88], [BBK88], [BB91], [BCS92]
Ref:	=1997A&A...328..499G
by	GUILLEMIN P. , BERGERON J.
	Astron. Astrophys., 328, 499-509 (1997)
	Evolution of quasar absorption-selected galaxies.
o	Tables 2, 3, 4, Figs 2, 3: <[GB97] HHMM+DDd GN> N=41
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GB98]
[GB98]	(Groenewegen+Blommaert, 1998)= (SMC)
Write:	<<[GB98] SNNa>>
N:	32
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1998A&A...332...25G
by	GROENEWEGEN M.A.T. , BLOMMAERT J.A.D.L.
	Astron. Astrophys., 332, 25-32 (1998)
	Near-infrared photometry and optical spectroscopy of IRAS sources in the Small Magellanic Cloud.
o	Table 1 : [GB98] S8 is IRAS F00468-7427, not -7341.
o	Table 2: <[GB98] SNNa> (Nos 1-19, 20a-20b, 21-31)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBA2007]
[GBA2007]	(Gudel+Briggs+Arzner+, 2007)
Write:	<<[GBA2007] NNNN>>
N:	2347
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Survey of the Taurus Molecular Cloud (TMC) using XMM-Newton: XEST survey, general survey format 'FF-NNN', also numbered 'NNNN'.
in source:	NAME TMC
Ref:	=2007A&A...468..353G
by	GUEDEL M. , BRIGGS K.R., ARZNER K., AUDARD M., BOUVIER J., FEIGELSON E.D., FRANCIOSINI E., GLAUSER A., GROSSO N., MICELA G., MONIN J.-L., MONTMERLE T., PADGETT D.L., PALLA F., PILLITTERI I., REBULL L., SCELSI L., SILVA B., SKINNER S.L., STELZER B., TELLESCHI A.
	Astron. Astrophys., 468, 353-377 (2007)
	The XMM-Newton extended survey of the Taurus Molecular Cloud (XEST).
o	Table 14, col.(1): <[GBA2007] NNNN> (Nos 1-2347) = Table 14, col.(2): <XEST FF-NNN> N=2347.
=E=	Catalogue in electronic form as J/A+A/468/353
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBA2014]
[GBA2014]	(Guennou+Biviano+Adami +, 2014)
Write:	<<[GBA2014] JHHMMSS.ss+DDMMSS.s>> <<[GBA2014] N.N>>
N:	137 (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Gemini GMOS observation of N=137 galaxies in the LCDCS 0504 cluster of galaxies. Use of archival HST ACS and VLT FORS 2 images.
in source:	LCDCS 0504
Ref:	=2014A&A...566A.149G
by	GUENNOU L. , BIVIANO A., ADAMI C., LIMOUSIN M., LIMA NETO G.B., MAMON G.A., ULMER M.P., GAVAZZI R., CYPRIANO E.S., DURRET F., CLOWE D., LEBRUN V., ALLAM S., BASA S., BENOIST C., CAPPI A., HALLIDAY C., ILBERT O., JOHNSTON D., JULLO E., JUST D., KUBO J.M., MARQUEZ I., MARSHALL P., MARTINET N., MAUROGORDATO S., MAZURE A., MURPHY K.J., PLANA H., ROSTAGNI F., RUSSEIL D., SCHIRMER M., SCHRABBACK T., SLEZAK E., TUCKER D., ZARITSKY D., ZIEGLER B.
	Astron. Astrophys., 566A, 149-149 (2014)
	Mass profile and dynamical status of the z ~ 0.8 galaxy cluster LCDCS 0504.
o	Table 2: <[GBA2014] JHHMMSS.ss+DDMMSS.s> N=137. Table 3: <[GBA2014] N.N> N=8.
=E=	Catalogue in electronic form as J/A+A/566/A149
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBA2017]
[GBA2017]	(Gonzalez-Lopez+Bauer+Aravena+, 2017)
Write:	<<[GBA2017] ANNNN-ELNN>> <<[GBA2017] MACSJHHMM-ELNN>> <<[GBA2017] AS1063-ELNN>>
N:	3+6+3+5+9
Object:	Em-line source (SIMBAD class: EmObj = Emission Object)
Stat:	is completely incorporated in Simbad
Note:	ALMA 1.1mm continuum observations of N=27 emission line candidates in N=5 galaxy clusters, as part of the Frontier Fields survey. See also [GBR2017].
in source:	ACO 2744
in source:	MCS J0416.1-2403
in source:	ClG J1149+2223
in source:	ACO 370
in source:	ACO S 1063
Ref:	=2017A&A...608A.138G
by	GONZALEZ-LOPEZ J. , BAUER F.E., ARAVENA M., LAPORTE N., BRADLEY L., CARRASCO M., CARVAJAL R., DEMARCO R., INFANTE L., KNEISSL R., KOEKEMOER A.M., MUNOZ ARANCIBIA A.M., TRONCOSO P., VILLARD E., ZITRIN A.
	Astron. Astrophys., 608A, 138-138 (2017)
	The ALMA Frontier Fields Survey. III. 1.1 mm emission line identifications in Abell 2744, MACSJ 0416.1-2403, MACSJ 1149.5+2223, Abell 370, and Abell S1063.
o	Tables 2-3: <[GBA2017] A2744-ELNN> (Nos 01-03), <[GBA2017] MACSJ0416-ELNN> (Nos 01-06), <[GBA2017] MACSJ1149-ELNN> (Nos 01-03), <[GBA2017] A370-ELNN> (Nos 01-05), <[GBA2017] AS1063-ELNN> (Nos 01-09).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBB2000]
[GBB2000]	(Gardner+Baum+Brown+, 2000)= (HDFS) = ([GBB2000a])
Write:	<<[GBB2000] NNNNN>> <<[GBB2000] HDFS JHHMMSS.ss+DDMMSS.s>>
N:	674
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST STIS observations of the HDFS.
in source:	NAME HDFS
Ref:	=2000AJ....119..486G
by	GARDNER J.P. , BAUM S.A., BROWN T.M., CAROLLO C.M., CHRISTENSEN J., DASHEVSKY I., DICKINSON M.E., ESPEY B.R., FERGUSON H.C., FRUCHTER A.S., GONNELLA A.M., GONZALEZ-LOPEZLIRA R.A., HOOK R.N., KAISER M.E., MARTIN C.L., SAHU K.C., SAVAGLIO S., SMITH T.E., TEPLITZ H.I., WILLIAMS R.E., WILSON J.
	Astron. J., 119, 486-508 (2000)
	The Hubble Deep Field South: STIS imaging.
o	Table 2: <[GBB2000] NNNNN> N=674 among (Nos 1-690, 10097-10173) = <[GBB2000] HDFS JHHMMSS.ss+DDMMSS.s> N=674.
=E=	Catalogue in electronic form as J/AJ/119/486
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBB2000a]
[GBB2000a]	(Gardner+Baum+Brown+, 2000)
*****	Avoid the usage of [GBB2000a], prefer [GBB2000]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBB2000b]
[GBB2000b]	(Gliozzi+Boller+Brinkmann+, 2000)
Write:	<<[GBB2000b] JHHMMSS.s+DDMMSS>>
N:	1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	N=1 X-ray source SW of PKS 0558-504.
Ref:	=2000A&A...356L..17G
by	GLIOZZI M. , BOLLER T., BRINKMANN W., BRANDT W.N.
	Astron. Astrophys., 356, 17-20 (2000)
	ROSAT HRI monitoring of X-ray variability in the NLS1 galaxy PKS 0558-504.
o	<[GBB2000b] JHHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBB2004]
[GBB2004]	(Gioia+Braito+Branchesi+, 2004)
Write:	<<[GBB2004] 1054-0321 N>> <<[GBB2004] JHHMMSS.s+DDMMSS>>
N:	3+1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton MOS2 image of ClG 1054-0321 = 1E 1054.4-0321: N=2 distinct components plus a fainter emission region (component 3) and a point source emission 'JHHMMSS.s+DDMMSS.s'.
in source:	ClG 1054-0321 = 1E 1054.4-0321
Ref:	=2004A&A...419..517G
by	GIOIA I.M. , BRAITO V., BRANCHESI M., DELLA CECA R., MACCACARO T., TRAN K.-V.
	Astron. Astrophys., 419, 517-525 (2004)
	An X-ray review of MS 1054-0321: Hot or not?
o	Fig.1, Table 2: <[GBB2004] 1054-0321 N> (Nos 1-3) = <[GBB2004] JHHMMSS.s+DDMMSS> N=2. Fig.1, Table 3: <[GBB2004] JHHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBB2006]
[GBB2006]	(Girardi+Boschin+Barrena, 2006)
Write:	<<[GBB2006] NN>>
N:	93
Object:	G in ClG (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spectroscopic data obtained at the TNG telescope combined with photometric data obtained at the INT telescope of the region of ACO 697.
in source:	ACO 697
Ref:	=2006A&A...455...45G
by	GIRARDI M. , BOSCHIN W., BARRENA R.
	Astron. Astrophys., 455, 45-59 (2006)
	Internal dynamics of the massive cluster Abell 697: a multiwavelength analysis.
o	Fig.1, Table 1: <[GBB2006] NN> (Nos 1-92).
=E=	Catalogue in electronic form as J/A+A/455/45
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBB2008]
[GBB2008]	(Girardi+ Barrena+Boschin+, 2008)
Write:	<<[GBB2008] NNN>>
N:	293
Object:	G in ClG (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	INT WFC photometry and TNG DOLORES spectroscopy of the field of ACO 520.
in source:	ACO 520 = 1E 0451.5+0250
Ref:	=2008A&A...491..379G
by	GIRARDI M. , BARRENA R., BOSCHIN W., ELLINGSON E.
	Astron. Astrophys., 491, 379-395 (2008)
	Cluster Abell 520: a perspective based on member galaxies. A cluster forming at the crossing of three filaments?
o	Table 1: <[GBB2008] NNN> (Nos 1-293).
=E=	Catalogue in electronic form as <J/A+A/491/379/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBB2010]
[GBB2010]	(Gouliermis+Bestenlehner+Brandner+, 2010)= ([GBB2010a])
Write:	<<[GBB2010] NNNN>>
N:	2506
Object:	* (SIMBAD class: Star)
Note:	VLT ISAAC observations of the star-forming region NGC 346/N66.
in source:	Magellanic Clouds:SMC:NGC 346 = NGC 346
in source:	Magellanic Clouds:SMC:LHA 115-N 66 = LHA 115-N 66
Ref:	=2010A&A...515A..56G
by	GOULIERMIS D.A. , BESTENLEHNER J.M., BRANDNER W., HENNING T.
	Astron. Astrophys., 515A, 56-56 (2010)
	Recent star formation at low metallicities. The star-forming region NGC 346/N66 in the Small Magellanic Cloud from near-infrared VLT/ISAAC observations.
o	Table 1: <[GBB2010] NNNN> (Nos 1-2506).
=E=	Catalogue in electronic form as J/A+A/515/A56
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBB2010a]
[GBB2010a]	(Gouliermis+Bestenlehner+Brandner+, 2010)
*****	Avoid the usage of [GBB2010a], prefer [GBB2010]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBB2010b]
[GBB2010b]	(Girardi+Boschin+Barrena+, 2010)
Write:	<<[GBB2010b] NN>>
N:	88
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	TNG DOLORES/MOS (spectroscopy) and INT WFC (photometry) observations of N=88 galaxies in Abell 2294.
in source:	ACO 2294
Ref:	=2010A&A...517A..65G
by	GIRARDI M. , BOSCHIN W., BARRENA R.
	Astron. Astrophys., 517A, 65-65 (2010)
	Internal dynamics of Abell 2294: a massive, likely merging cluster.
o	Table 1: <[GBB2010b] NN> (Nos 1-88).
=E=	Catalogue in electronic form as <J/A+A/517/A65/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBB2011]
[GBB2011]	(Gutierrez+Beckman+Buenrostro, 2011)= ([GBB2011a])
Write:	<<[GBB2011] M51 NNNN>> <<[GBB2011] NGC 4449 NNN>>
N:	2659+273
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	HST ACS Hα observations of HII regions in M51 and NGC 4449.
in source:	M 51 = NGC 5194
in source:	NGC 4449
Ref:	=2011AJ....141..113G
by	GUTIERREZ L. , BECKMAN J.E., BUENROSTRO V.
	Astron. J., 141, 113 (2011)
	Properties of the HII region populations of M51 and NGC 4449 from Hα images with the Advanced Camera for Surveys on the Hubble Space Telescope.
o	Table 2: <[GBB2011] M51 NNNN> (Nos 1-2659). Table 3: <[GBB2011] NGC4449 NNN> (Nos 1-273).
=E=	Catalogue in electronic form as <J/AJ/141/113/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBB2011a]
[GBB2011a]	(Gutierrez+Beckman+Buenrostro, 2011)
*****	Avoid the usage of [GBB2011a], prefer [GBB2011]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBB2011b]
[GBB2011b]	(Girardi+Bardelli+Barrena+, 2011)
Write:	<<[GBB2011b] NNN>>
N:	128
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	TNG DOLORES spectroscopy and INT WFC g'r'i' photometry of N=128 galaxies in the field of Abell 2254.
in source:	ACO 2254
Ref:	=2011A&A...536A..89G
by	GIRARDI M. , BARDELLI S., BARRENA R., BOSCHIN W., GASTALDELLO F., NONINO M.
	Astron. Astrophys., 536A, 89-89 (2011)
	Internal dynamics of Abell 2254: a merging galaxy cluster with a clumpy, diffuse radio emission.
o	Table 1: <[GBB2011b] NNN> (Nos 1-128).
=E=	Catalogue in electronic form as J/A+A/536/A89
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBB2012]
[GBB2012]	(Gennaro+Bik+Brandner+, 2012)
Write:	<<[GBB2012] EN>> <<[GBB2012] YN>> <<[GBB2012] AGBN>> <<[GBB2012] RGN>>
N:	13 (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	NTT/SofI deep JHKS photometry and long slit K band spectroscopy of the brightest members of the [CWP2007] CN15/16/17 molecular complex.
Ref:	=2012A&A...542A..74G
by	GENNARO M. , BIK A., BRANDNER W., STOLTE A., ROCHAU B., BEUTHER H., GOULIERMIS D., TACKENBERG J., KUDRYAVTSEVA N., HUSSMANN B., SCHULLER F., HENNING Th.
	Astron. Astrophys., 542A, 74-74 (2012)
	Multiple episodes of star formation in the CN15/16/17 molecular complex.
o	Table 2 : <[GBB2012] EN> (Nos E1-E4), <[GBB2012] YN> (Nos Y1-Y4), <[GBB2012] AGBN> (No AGB1), <[GBB2012] RGN> (Nos RG1-RG4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GBC
GBC	(Green Bank Cloud)= ([CLH2011])
Write:	<<GBC JHHMMSS.s+DDMMSS>>
N:	13
Object:	HI Cloud (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	Green Bank Telescope survey of nearby galaxy groups, searching for neutral hydrogen clouds.
Ref:	=2011AJ....141....9C
by	CHYNOWETH K.M. , LANGSTON G.I., HOLLEY-BOCKELMANN K.
	Astron. J., 141, 9 (2011)
	H I clouds in the M81 filament as dark matter minihalos–a phase-space mismatch.
o	Table 1, col(1): <[CLH2011] N> (Nos 1-5). Table 1, col(2): <GBC JHHMMSS.s+DDMMSS> N=13. Vanderbilt University
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
History	of this Acronym: replaces [CLH2011] (for format JHHMMSS.s+DDMMSS)
Details on Acronym: [GBC2001]
[GBC2001]	(Ganguly+Bond+Charlton+, 2001) (Not yet in Simbad)
Write:	<<[GBC2001] Group N>>
N:	5
Object:	Group (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=5 clusters of QSOs.
Ref:	=2001ApJ...549..133G
by	GANGULY R. , BOND N.A., CHARLTON J.C., ERACLEOUS M., BRANDT W.N., CHURCHILL C.W.
	Astrophys. J., 549, 133-154 (2001)
	On the origin of intrinsic narrow absorption lines in z≲1 QSOs.
o	Table 6: <[GBC2001] Group N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBC2004]
[GBC2004]	(Garg+Blondin+Challis+, 2004)= ([GBC2004a])
Write:	<<[GBC2004] JHHMMSS.ss+DDMMSS.s>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Cerro Tololo 4m observations. Host galaxies of SN 2004GA and SN 2004GB.
Ref:	=2004IAUC.8439....2G
by	GARG A. , BLONDIN S., CHALLIS P., STUBBS C., (The SuperMACHO Collaboration), AGUILERA C., PRIETO J.L., BRAMICH D., HUBER M., MINNITI D.
	IAU Circ., 8439, 2-None (2004)
	Supernovae 2004ga and 2004gb.
o	<[GBC2004] JHHMMSS.ss+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBC2004a]
[GBC2004a]	(Garg+Blondin+Challis+, 2004)
*****	Avoid the usage of [GBC2004a], prefer [GBC2004]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBC2004b]
[GBC2004b]	(Gratton+Bragaglia+Clementini, 2004)
*****	Avoid the usage of [GBC2004b], prefer [DCM2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBC2009]
[GBC2009]	(Gonzales Hernandez+Bonifacio+Caffau+, 2009)
Write:	<<[GBC2009] AAANNNNNN>>
N:	79+84
Object:	* (SIMBAD class: Star)
Note:	VLT FLAMES GIRAFFE observations of a sample of N=84 SG (subgiant branch) and N=79 MS (main sequence) stars in NGC 6397.
in source:	NGC 6397
Ref:	=2009A&A...505L..13G
by	GONZALEZ HERNANDEZ J.I. , BONIFACIO P., CAFFAU E., STEFFEN M., LUDWIG H.-G., BEHARA N.T., SBORDONE L., CAYREL R., ZAGGIA S.
	Astron. Astrophys., 505L, 13-16 (2009)
	Lithium in the globular cluster NGC 6397. Evidence for dependence on evolutionary status.
o	Table 2: <[GBC2009] AAANNNNNN> N=79+84 among (Nos MSS001253-049487, SGB001167-036901).
=E=	Catalogue in electronic form as J/A+A/505/L13
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBC2010]
[GBC2010]	(Gomez+Baes+Cortese+, 2010) (Not yet in Simbad)
Write:	<<[GBC2010] M86-W>> <<[GBC2010] M86-off>> <<[GBC2010] lane>>
N:	4
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	Herschel SPIRE 250-500µm observations of M86.
in source:	NGC 4406 = M 86
Ref:	=2010A&A...518L..45G
by	GOMEZ H.L. , BAES M., CORTESE L., SMITH M.W.L., BOSELLI A., CIESLA L., BENDO G.J., POHLEN M., DI SEREGO ALIGHIERI S., AULD R., BARLOW M.J., BOCK J.J., BRADFORD M., BUAT V., CASTRO-RODRIGUEZ N., CHANIAL P., CHARLOT S., CLEMENTS D.L., COORAY A., CORMIER D., DAVIES J.I., DWEK E., EALES S., ELBAZ D., GALAMETZ M., GALLIANO F., GEAR W.K., GLENN J., GRIFFIN M., HONY S., ISAAK K.G., LEVENSON L.R., LU N., MADDEN S., O'HALLORAN B., OKUMURA K., OLIVER S., PAGE M.J., PANUZZO P., PAPAGEORGIOU A., PARKIN T.J., PEREZ-FOURNON I., RANGWALA N., RIGBY E.E., ROUSSEL H., RYKALA A., SACCHI N., SAUVAGE M., SCHIRM M.R.P., SCHULZ B., SPINOGLIO L., SRINIVASAN S., STEVENS J.A., SYMEONIDIS M., TRICHAS M., VACCARI M., VIGROUX L., WILSON C.D., WOZNIAK H., WRIGHT G.S., ZEILINGER W.W.
	Astron. Astrophys., 518L, 45-45 (2010)
	The dust morphology of the elliptical galaxy M86 with SPIRE.
o	Fig. 1: <[GBC2010] M86-W> (Nos M86-N, M86-S), <[GBC2010] M86-off> N=1, <[GBC2010] lane> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBC2019]
[GBC2019]	(Graham+Brown+Chadwick, 2019)
Write:	<<[GBC2019] PS JHHMM.m+DDMM>>
N:	9
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	N=9 point sources in the field of IC 310, using 8 yr of data from the Fermi Large Area Telescope (Fermi LAT) between 100MeV and 500 GeV.
in source:	IC 310
Ref:	=2019MNRAS.485.3277G
by	GRAHAM J.A. , BROWN A.M., CHADWICK P.M.
	Mon. Not. R. Astron. Soc., 485, 3277-3287 (2019)
	Fermi-LAT observations of extreme spectral variability in IC 310.
o	Table 1: <[GBC2019] PS JHHMM.m+DDMM> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBD2020]
[GBD2020]	(Girardi+Boschin+De Grandi+, 2020)
Write:	<<[GBD2020] NNN>>
N:	285
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	TNG DOLORES/MOS spectroscopy of N=285 galaxies in the Lyra complex.
in source:	NAME Lyra Complex
Ref:	=2020A&A...633A.108G
by	GIRARDI M. , BOSCHIN W., DE GRANDI S., LONGHETTI M., CLAVICO S., ECKERT D., GASTALDELLO F., GHIZZARDI S., NONINO M., ROSSETTI M.
	Astron. Astrophys., 633A, 108-108 (2020)
	The velocity field of the Lyra complex.
o	Table 1: <[GBD2020] NNN> (Nos 1-285).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBE2018]
[GBE2018]	(Gilbank+Barrientos+Ellingson+, 2018) (Not yet in Simbad)
Write:	<<[GBE2018] JHHMMSS+DDMM.mA>> <<[GBE2018] JDDD.dddddd+DD.dddddd>>
N:	6+21
Object:	Cluster of G + BCG (SIMBAD class: Galaxy)
Note:	Follow-up observations of galaxy clusters from the first Red-sequence Cluster Survey (RCS-1) revealing N=3 spectroscopic pairs and N=21 BCGs. Use of CFHT MOS, WHT LDSS2, VLT FOR2/MXU, Gemini South GMOS, Keck DEIMOS and Subaru FOCAS data.
Ref:	=2018MNRAS.476.1991G
by	GILBANK D.G. , BARRIENTOS L.F., ELLINGSON E., BLINDERT K., YEE H.K.C., ANGUITA T., GLADDERS M.D., HALL P.B., HERTLING G., INFANTE L., YAN R., CARRASCO M., GARCIA-VERGARA C., DAWSON K.S., LIDMAN C., MOROKUMA T.
	Mon. Not. R. Astron. Soc., 476, 1991-2012 (2018)
	Spectroscopic characterization of galaxy clusters in RCS-1: spectroscopic confirmation, redshift accuracy, and dynamical mass-richness relation.
o	Tables 1-2: <RCS JHHMMSS+DDMM.m> N=25+21. Table 1: <[GBE2018] JHHMMSS+DDMM.mA> N=6. Table 3: <[GBE2018] JDDD.dddddd+DD.dddddd> N=21.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBG2016]
[GBG2016]	(Girardi+Boschin+Gastaldello+, 2016)
Write:	<<[GBG2016] NNN>>
N:	132
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	TNG DOLORES/MOS spectroscopic and INT WFC photometric observations of N=132 galaxies in the field of ACO 523.
in source:	ACO 523
Ref:	=2016MNRAS.456.2829G
by	GIRARDI M. , BOSCHIN W., GASTALDELLO F., GIOVANNINI G., GOVONI F., MURGIA M., BARRENA R., ETTORI S., TRASATTI M., VACCA V.
	Mon. Not. R. Astron. Soc., 456, 2829-2847 (2016)
	A multiwavelength view of the galaxy cluster Abell 523 and its peculiar diffuse radio source.
o	Table 2: <[GBG2016] NNN> (Nos 1-132).
=E=	Catalogue in electronic form as J/MNRAS/456/2829
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBG2023]
[GBG2023]	(Grazian+Boutsia+Giallongo+, 2023) (Not yet in Simbad)
Write:	<<[GBG2023] UDeep NNNNNN>> <<[GBG2023] Wide NNNNNN>>
N:	8+14
Object:	QSO + Poss. QSO (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=3+5 confirmed and candidate QSOs in the Subaru HSC-Ultradeep survey, N=8+6 confirmed and candidate QSOs in the HSC-Wide survey, as part of the RUBICON (Reionizing the Universe with Bright Cosmological Nuclei) survey. Use of the Third Public Data Release of the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP PDR3).
Ref:	=2023ApJ...955...60G
by	GRAZIAN A. , BOUTSIA K., GIALLONGO E., CRISTIANI S., FONTANOT F., BISCHETTI M., BONGIORNO A., CALDERONE G., CUPANI G., D'ODORICO V., FERUGLIO C., FIORE F., GUARNERI F., PORRU M., SACCHEO I.
	Astrophys. J., 955, 60 (2023)
	Crossing the Rubicon of Reionization with z ~ 5 QSOs.
o	Table 1: <[GBG2023] UDeep NNNNNN> N=8 among (Nos 258-233735). Table 2: <[GBG2023] Wide NNNNNN> N=14 among (Nos 18331-220671).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [GBH2005]
[GBH2005]	(Giveon+Becker+Helfand+, 2005)= ([GBH2005a])
Write:	<<[GBH2005] GLLL.lllll+L.lllll>>
N:	687
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	VLA galactic plane catalogs and MSX6C catalogue are used to search for ultra-compact HII regions. See also paper II: [GBH2005b]
Ref:	=2005AJ....129..348G
by	GIVEON U. , BECKER R.H., HELFAND D.J., WHITE R.L.
	Astron. J., 129, 348-354 (2005)
	A new catalog of radio compact H II regions in the Milky Way.
o	Table 4: <[GBH2005] GLLL.lllll+L.lllll> N=687.
=E=	Catalogue in electronic form as J/AJ/129/348
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBH2005a]
[GBH2005a]	(Giveon+Becker+Helfand+, 2005)
*****	Avoid the usage of [GBH2005a], prefer [GBH2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBH2005b]
[GBH2005b]	(Giveon+Becker+Helfand+, 2005)
Write:	<<[GBH2005b] GLLL.lllll+L.lllll>>
N:	556
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA catalogue at 1.4GHz of the galactic plane region in conjunction with the MSX6C catalogue. See also paper I: [GBH2005].
Ref:	=2005AJ....130..156G
by	GIVEON U. , BECKER R.H., HELFAND D.J., WHITE R.L.
	Astron. J., 130, 156-164 (2005)
	A new catalog of radio compact H II regions in the Milky way. II. The 1.4 GHz data.
o	Table 4: <[GBH2005b] GLLL.lllll+L.lllll> N=556.
=E=	Catalogue in electronic form as J/AJ/130/156
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBH2021]
[GBH2021]	(Ghirardini+Bulbul+Hoang +, 2021)
Write:	<<[GBH2021] Supercluster>> <<[GBH2021] RSE>> <<[GBH2021] RN>> <<[GBH2021] A>>
N:	1+1+1+5
Object:	Supercluster + (Rad) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=1 supercluster discovered in the eROSITA Final Equatorial Depth Survey (eFEDS). LOFAR and uGMRT observations of N=2+5 extended and discrete radio sources respectively in the supercluster.
Ref:	=2021A&A...647A...4G
by	GHIRARDINI V. , BULBUL E., HOANG D.N., KLEIN M., OKABE N., BIFFI V., BRUGGEN M., RAMOS-CEJA M.E., COMPARAT J., OGURI M., SHIMWELL T.W., BASU K., BONAFEDE A., BOTTEON A., BRUNETTI G., CASSANO R., DE GASPERIN F., DENNERL K., GATUZZ E., GASTALDELLO F., INTEMA H., MERLONI A., NANDRA K., PACAUD F., PREDEHL P., REIPRICH T.H., ROBRADE J., ROTTGERING H., SANDERS J., VAN WEEREN R.J., WILLIAMS W.L.
	Astron. Astrophys., 647A, 4-4 (2021)
	Discovery of a supercluster in the eROSITA Final Equatorial Depth Survey: X-ray properties, radio halo, and double relics.
o	<[GBH2021] Supercluster> N=1. Fig. 6, Table 6: <[GBH2021] RSE> N=1, <[GBH2021] RNE> N=1, <[GBH2021] A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBH81]
[GBH81]	(Gatley+Becklin+Hyland+, 1981)
Write:	<<[GBH81] FS>> <<[GBH81] PS>>
N:	2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	NIR study of the HII region LHA 120-N 159 in the LMC. N=1 foreground star (FS) and N=1 protostar (PS) are found.
in source:	Magellanic Clouds:LMC:LHA 120-N 159 = LHA 120-N 159
Ref:	=1981MNRAS.197p..17G
by	GATLEY I. , BECKLIN E.E., HYLAND A.R., JONES T.J.
	Mon. Not. R. Astron. Soc., 197, part no 16, 17-21 (1981)
	Discovery of a protostar in the Large Magellanic Cloud.
o	Table 1: <[GBH81] AA> (Nos FS, PS).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBH97]
[GBH97]	(Greiner+Bade+Hurley+, 1997)
Write:	<<[GBH97] PNN>> <<[GBH97] SNN>>
N:	20+29
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC (Nos P1-P20) and All-Sky-Survey (Nos S1-S29) observations.
Ref:	=1997A&A...325..640G
by	GREINER J. , BADE N., HURLEY K., KIPPEN R.M., LAROS J.
	Astron. Astrophys., 325, 640-646 (1997)
	Rapid follow-up ROSAT observation of GRB 940301.
o	Table 2: <[GBH97] PNN> (Nos P1-P20). Table 3: <[GBH97] SNN> (Nos S1-S29).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBJ2000]
[GBJ2000]	(Garnavich+Barmby+Jha+, 2000)
Write:	<<[GBJ2000] Star A>>
N:	4
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=4 comparison stars in the field of GRB 000301C.
Ref:	=2000GCN...573....1G
by	GARNAVICH P. , BARMBY P., JHA S., STANEK K.
	GRB Coordinates Network, Circular Service, 573, 1-None (2000)
	GRB000301C, optical observations.
o	<[GBJ2000] Star A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBJ2012]
[GBJ2012]	(Grutzbauch+Bauer+Jorgensen+, 2012)
Write:	<<[GBJ2012] NNN>>
N:	201
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Gemini-North NIRI observations of N=201 objects in the field of the galaxy cluster XDCP J2235.3-2557.
in source:	ClG J2235-2557 = XDCP J2235.3-2557
Ref:	=2012MNRAS.423.3652G
by	GRUTZBAUCH R. , BAUER A.E., JORGENSEN I., VARELA J.
	Mon. Not. R. Astron. Soc., 423, 3652-3662 (2012)
	Suppression of star formation in the central 200 kpc of a z= 1.4 galaxy cluster.
o	Tables 1-2: <[GBJ2012] NNN> (Nos 1-201).
=E=	Catalogue in electronic form as <J/MNRAS/423/3652/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBK2001]
[GBK2001]	(Ge+Bechtold+Kulkarni, 2001)
Write:	<<[GBK2001] QSO J1234+0758 abs N.NN>> <<[GBK2001] QSO J1234+0758 abs N.NNNN>>
N:	1+3
Object:	DLA
Note:	Observations with the Blue Channel Spectrograph on MMT. N=1 DLA in the line of sight of QSO B1232+0815 = QSO J1234+0758, divided in 3 components.
Ref:	=2001ApJ...547L...1G
by	GE J. , BECHTOLD J., KULKARNI V.P.
	Astrophys. J., 547, 1-5 (2001)
	H_{2}, C I, metallicity, and dust depletion in the z = 2.34 damped Lyα absorption system toward QSO 1232+0815.
o	QSO 1232+0815 = QSO J1234+0758
o	<[GBK2001] QSO J1234+0758 abs N.NN> N=1, <[GBK2001] QSO J1234+0758 abs N.NNNN> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBK2004]
[GBK2004]	(Garnavich+Bonanos+Krisciunas+, 2004) (Not yet in Simbad)
Write:	<<[GBK2004] NN>>
N:	10
Object:	* (SIMBAD class: Star)
Note:	N=10 local standard stars.
Ref:	=2004ApJ...613.1120G
by	GARNAVICH P.M. , BONANOS A.Z., KRISCIUNAS K., JHA S., KIRSHNER R.P., SCHLEGEL E.M., CHALLIS P., MACRI L.M., HATANO K., BRANCH D., BOTHUN G.D., FREEDMAN W.L.
	Astrophys. J., 613, 1120-1132 (2004)
	The luminosity of SN 1999by in NGC 2841 and the nature of ``Peculiar'' type Ia supernovae.
o	Fig.1, Table 1: <[GBK2004] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBK2010]
[GBK2010]	(Goddard+Bastian+Kennicutt, 2010)
Write:	<<[GBK2010] NNN>>
N:	276
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	N=276 clusters in the merger galaxy NGC 3256. Use of archival HST ACS images.
in source:	NGC 3256
Ref:	=2010MNRAS.405..857G
by	GODDARD Q.E. , BASTIAN N., KENNICUTT R.C.
	Mon. Not. R. Astron. Soc., 405, 857-869 (2010)
	On the fraction of star clusters surviving the embedded phase.
o	Table 5: <[GBK2010] NNN> (Nos 1-276).
=E=	Catalogue in electronic form as <J/MNRAS/405/857/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBK2011]
[GBK2011]	(Goddard+Bresolin+Kennicutt+, 2011)
Write:	<<[GBK2011] NNNa>> <<[GBK2011] NNN.NNNN>>
N:	34
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Subaru FOCAS observations of N=34 HII regions in the extended ultraviolet disc of NGC 4625.
in source:	NGC 4625
Ref:	=2011MNRAS.412.1246G
by	GODDARD Q.E. , BRESOLIN F., KENNICUTT R.C., RYAN-WEBER E.V., ROSALES-ORTEGA F.F.
	Mon. Not. R. Astron. Soc., 412, 1246-1258 (2011)
	On the nature of the H II regions in the extended ultraviolet disc of NGC 4625.
o	Table 1: <[GBK2011] NNNa> N=30 among (Nos 103-223), <[GBK2011] NNN.NNN> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBK2017]
[GBK2017]	(Getman+Broos+Kuhn+, 2017)
Write:	<<[GBK2017] GLLL.llll+BB.bbbb>>
N:	1638654
Object:	(MIR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	The SFiNCs (Star Formation in Nearby Clouds) IRAC source catalog. This catalog covers the 22 SFiNCs star forming regions and their vicinities on the sky, and comprises 1638654 IRAC sources. This catalog retains all point sources with the photometric signal-to-noise ratio >5 in both [3.6] and [4.5] channels. See also SPCM.
Ref:	=2017ApJS..229...28G
by	GETMAN K.V. , BROOS P.S., KUHN M.A., FEIGELSON E.D., RICHERT A.J.W., OTA Y., BATE M.R., GARMIRE G.P.
	Astrophys. J., Suppl. Ser., 229, 28-28 (2017)
	Star Formation in Nearby Clouds (SFiNCs): X-ray and infrared source catalogs and membership.
o	<NAME ONC Flank W> (Nos S, N). Table 6: <[GBK2017] GLLL.llll+BB.bbbb> N=1638654. Tables 7-8: <SPCM JHHMMSS.ss+DDMMSS.s> N=8492.
=E=	Catalogue in electronic form as <J/ApJS/229/28/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GBL
GBL	(GAMBLES)
Write:	<<GBL JHHMM+DDMM>> <<GBL HHMM+DDMM>> (not recognised by Simbad, but found in literature)
N:	8660
Object:	? (SIMBAD class: _Candidate = Double or Multiple Star Candidate)
Note:	The Gaia Assorted Mass Binaries Long Excluded from SloWPoKES (GAMBLES) comprises N=8660 statistically significant wide pairs, available in a living online database (https://filtergraph.com/gambles).
Ref:	=2017AJ....153..259O
by	OELKERS R.J. , STASSUN K.G., DHITAL S.
	Astron. J., 153, 259-259 (2017)
	Gaia Assorted Mass Binaries Long Excluded from SLoWPoKES (GAMBLES): identifying ultra-wide binary pairs with components of diverse mass.
o	(Erratum) erratum vol. 154, art.174 (2017)
o	<GBL JHHMM+DDMM> N=8660.
=E=	Catalogue in electronic form as <J/AJ/153/259/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GBL2009]
[GBL2009]	(Godfrey+Bicknell+Lovell+, 2009) (Not yet in Simbad)
Write:	<<[GBL2009] HSN>> <<[GBL2009] JN>>
N:	2+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Long Baseline Array observations of PKS 1421-490.
Ref:	=2009ApJ...695..707G
by	GODFREY L.E.H. , BICKNELL G.V., LOVELL J.E.J., JAUNCEY D.L., GELBORD J., SCHWARTZ D.A., MARSHALL H.L., BIRKINSHAW M., GEORGANOPOULOS M., MURPHY D.W., PERLMAN E.S., WORRALL D.M.
	Astrophys. J., 695, 707-723 (2009)
	A multiwavelength study of the high surface brightness hot spot in PKS 1421-490.
o	Fig. 3: <[GBL2009] HSN> (Nos HS1, HS2), <[GBL2009] JN> (No. J1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBM2002]
[GBM2002]	(Garay+Brooks+Mardones+, 2002)
Write:	<<[GBM2002] IRAS 15596-5301 A>> <<[GBM2002] JHHMMSS.s+DDMMSS.s>> <<[GBM2002] JHHMMSS.s+DDMMSS>> <<[GBM2002] JHHMMSS.ss+DDMMSS.s>>
N:	3+1+2+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA, SEST and MSX observations. Radio continuum emission observations toward 2 IRAS sources. N=3 compact radio-sources (Nos A-C) toward IRAS 15596-5301. N=1 peak of emission toward IRAS 16272-4837, 'J183035.0-484047.6' N=2 millimeter peaks 'J160332.9-530920' and 'J163058.7-484335' and N=1 MSX object seen in emission 'J163058.18-484347.9'.
in source:	IRAS 15596-5301
in source:	IRAS 16272-4837
Ref:	=2002ApJ...579..678G
by	GARAY G. , BROOKS K.J., MARDONES D., NORRIS R.P., BURTON M.G.
	Astrophys. J., 579, 678-687 (2002)
	Two massive star-forming regions at early evolutionary stages.
o	Parag. 3.4 : MSX object = EQ J163058-484347
o	Fig.1, Table 1: <[GBM2002] IRAS 15596-5301 A> (Nos A-C). Text: <[GBM2002] JHHMMSS.s+DDMMSS.s> N=1, <[GBM2002] JHHMMSS.s+DDMMSS> N=2, <[GBM2002] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBM2003]
[GBM2003]	(Garay+Brooks+Mardones+, 2003)
Write:	<<[GBM2003] IRAS 16547-4247 W>> <<[GBM2003] IRAS 16547-4247 W-WW>> <<[GBM2003] JHHMMSS.ss+DDMMSS.s>>
N:	4+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA and SEST observations. Radio continuum emission toward IRAS 16547-4247. N=3 sources (N, C, S) + 1 observed only at 8.6GHz (C-SE). N=1 em. mm peak 'J165817.24-425203.8' observed at 1.2mm. See also [RGB2005].
in source:	IRAS 16547-4247
Ref:	=2003ApJ...587..739G
by	GARAY G. , BROOKS K.J., MARDONES D., NORRIS R.P.
	Astrophys. J., 587, 739-747 (2003)
	A triple radio continuum source associated with IRAS 16547-4247: a collimated stellar wind emanating from a massive protostar.
o	PKS 1612-52 not identified.
o	Table 1: <[GBM2003] IRAS 16547-4247 W> (Nos N, C, S), <[GBM2003] IRAS 16547-4247 W-WW> (No. C-SE). Text: <[GBM2003] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBM2006]
[GBM2006]	(Garay+Brooks+Mardones+, 2006)
Write:	<<[GBM2006] HHMMm+DDMM>> <<[GBM2006] HHMMm+DDMMA>> <<[GBM2006] HHMMm+DDMMa>>
N:	25
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA observations: search for radio sources in 15 IRAS point sources.
Ref:	=2006ApJ...651..914G
by	GARAY G. , BROOKS K.J., MARDONES D., NORRIS R.P.
	Astrophys. J., 651, 914-932 (2006)
	A multiwavelength study of young massive star-forming regions. I. The ionized gas content.
o	Figs, Table 2: <[GBM2006] HHMMm+DDMM>, <[GBM2006] HHMMm+DDMMA>, <[GBM2006] HHMMm+DDMMa>, N=25.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBM2007]
[GBM2007]	(Gosling+Bandyopadhyay+Miller-Jones+, 2007)
Write:	<<[GBM2007] a>>
N:	2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT-ISAAC detection of 2 candidate counterparts to the bursting pulsar GRO J1744-28.
Ref:	=2007MNRAS.380.1511G
by	GOSLING A.J. , BANDYOPADHYAY R.M., MILLER-JONES J.C.A., FARRELL S.A.
	Mon. Not. R. Astron. Soc., 380, 1511-1520 (2007)
	GRO J1744-28, search for the counterpart: infrared photometry and spectroscopy.
o	Fig.1, paragr. 3.1: <[GBM2007] a> (Nos a-b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBM2008]
[GBM2008]	(Gezari+Basa+Martin+, 2008)= (GALEX)
Write:	<<[GBM2008] DN-NN>> <<[GBM2008] GALEX JHHMMSS.s+DDMMSS>>
N:	87
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	GALEX UV and CFHTLS Deep Imaging Surveys data of UV variable sources.
Ref:	=2008ApJ...676..944G
by	GEZARI S. , BASA S., MARTIN D.C., BAZIN G., FORSTER K., MILLIARD B., HALPERN J.P., FRIEDMAN P.G., MORRISSEY P., NEFF S.G., SCHIMINOVICH D., SEIBERT M., SMALL T., WYDER T.K.
	Astrophys. J., 676, 944-969 (2008)
	UV/Optical detections of candidate tidal disruption events by GALEX and CFHTLS.
o	Table 2: <[GBM2008] DN-NN> N=23+23+32+9 = <[GBM2008] GALEX JHHMMSS.s+DDMMSS> N=87.
=E=	Catalogue in electronic form as <J/ApJ/676/944/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBM2012]
[GBM2012]	(Giannetti+Brand+Massi+, 2012)
Write:	<<[GBM2012] A>>
N:	14 (SIMBAD class: MolCld = Molecular Cloud)
Note:	SEST CO, CS, H2CO, CN, CH3CCH, and SiO observations of Galactic HII region G353.2+0.9.
in source:	GAL 353.19+00.91
Ref:	=2012A&A...538A..41G
by	GIANNETTI A. , BRAND J., MASSI F., TIEFTRUNK A., BELTRAN M.T.
	Astron. Astrophys., 538A, 41-41 (2012)
	Molecular clouds under the influence of massive stars in the Galactic HII region G353.2+0.9.
o	Tables 2,4-6 : <[GBM2012] A> N=14 among [GBM2012] A- [GBM2012] P
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBM2015]
[GBM2015]	(Graur+Bianco+Modjaz, 2015)
Write:	<<[GBM2015] SDSS NNNN-NNNNN-NNN SN>>
N:	107
Object:	SN (SIMBAD class: Supernova = SuperNova)
Stat:	is completely incorporated in Simbad
Note:	N=107 supernovae discovered in SDSS DR9 galaxy spectra.
Ref:	=2015MNRAS.450..905G
by	GRAUR O. , BIANCO F.B., MODJAZ M.
	Mon. Not. R. Astron. Soc., 450, 905-925 (2015)
	A unified explanation for the supernova rate-galaxy mass dependence based on supernovae detected in Sloan galaxy spectra.
o	Table 1 : no coordinates are provided for the SNe; ingested in SIMBAD with the coordinates of the Galaxy truncated to 1''.
o	Table 1: <[GBM2015] SDSS NNNN-NNNNN-NNN SN> N=107.
=E=	Catalogue in electronic form as <J/MNRAS/450/905/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBM2019]
[GBM2019]	(Goldman+Boyer+Mcquinn+, 2019) (Not yet in Simbad)
Write:	<<[GBM2019] NNNN>>
N:	38
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Spitzer IRAC and HST WFC3 observations of N=38 sources in the field of the dwarf galaxy Leo P.
in source:	NAME Leo P
Ref:	=2019ApJ...884..152G
by	GOLDMAN S.R. , BOYER M.L., McQUINN K.B.W., SLOAN G.C., McDONALD I., VAN LOON J.T., ZIJLSTRA A.A., HIRSCHAUER A.S., SKILLMAN E.D., SRINIVASAN S.
	Astrophys. J., 884, 152-152 (2019)
	Asymptotic giant branch stars in the nearby dwarf galaxy Leo P.
o	Tables 2-3: <[GBM2019] NNNN> N=38 among (Nos 162049).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBM2021]
[GBM2021]	(Gim+Borthakur+Momjian+, 2021)
Write:	<<[GBM2021] M100 AHC N>>
N:	2
Object:	HI Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	VLA observations of N=2 anomalous HI clouds (AHCs) in M100, as part of the Deciphering the Interplay between the Interstellar medium, Stars, and the Circumgalactic medium (DIISC) survey in HI 21cm.
in source:	NGC 4321 = M 100
Ref:	=2021ApJ...922...69G
by	GIM H.B. , BORTHAKUR S., MOMJIAN E., PADAVE M., JANSEN R.A., NELSON D., HECKMAN T.M., KENNICUTT R.C.Jr, FOX A.J., PINEDA J.L., THILKER D., KAUFFMANN G., TUMLINSON J.
	Astrophys. J., 922, 69-69 (2021)
	DIISC-I: the discovery of kinematically anomalous H I clouds in M 100.
o	Fig. 4, Table 3: <[GBM2021] M100 AHC N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBM74]
[GBM74]	(Gatley+Becklin+Matthews+, 1974)= (IRS)
Write:	<<[GBM74] IRS N>> <<[GBM74] IRS N-W>>
N:	7
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	OMC:OMC 2 = OMC 2
Ref:	=1974ApJ...191L.121G
by	GATLEY I. , BECKLIN E.E., MATTHEWS K., NEUGEBAUER G., PENSTON M.V., SCOVILLE N.
	Astrophys. J., 191, 121-125 (1974)
	A new IR complex and molecular cloud in Orion.
o	<OMC 2>. Fig. 2: <[GBM74] IRS N> N=5
Ref:	=1986ApJ...311..360P
by	PENDLETON Y. , WERNER M.W., CAPPS R., LESTER D.
	Astrophys. J., 311, 360-370 (1986)
	Infrared reflection nebulae in Orion Molecular Cloud 2.
o	Table 1: <[GBM74] IRS N-W> Nos 4-N and 4-S
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBM90]
[GBM90]	(Goodman+Bastien+Myers+, 1990)= (G)
Write:	<<[GBM90] L1506 NN>> <<[GBM90] L1755 NN>> <<[GBM90] Per NN>>
N:	40+51+88
Object:	* (SIMBAD class: Star)
Note:	Stars in star-forming regions near LDN 1506, LDN 1755, and the complex of dark clouds in Perseus.
in source:	LDN 1506
in source:	LDN 1755
in source:	NAME Perseus Molecular Cloud
Ref:	=1990ApJ...359..363G
by	GOODMAN A.A. , BASTIEN P., MYERS P.C., MENARD F.
	Astrophys. J., 359, 363-377 (1990)
	Optical polarization maps of star-forming regions in Perseus, Taurus and Ophiuchus.
o	Table 1: <[GBM90] L1506 NN> (Nos 1-40). Table 2: <[GBM90] L1755 NN> (Nos 1-51). Table 3: <[GBM90] Per NN> (Nos 1-88).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBM92]
[GBM92]	(Garilli+Bottini+Maccagni+, 1992)
Write:	<<[GBM92] Cl 0043-25 A>> <<[GBM92] ACO 3186 A>> <<[GBM92] ACO S 400 A>> <<[GBM92] Cl 0043-25 NN>> <<[GBM92] ACO 3186 NN>> <<[GBM92] ACO S 400 NNN>>
N:	8+8+6+86+99+224
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Table 3, Spectroscopic results: format 'Cl 0043-25 A', (Nos A-H), N=8. format 'ACO 3186 A', (Nos A-H), N=8. format 'ACO S 400 A', (Nos A-F), N=6. Table 5 (a): format 'Cl 0043-25 NN', N=86 G. Table 5 (b): format 'ACO 3186 NN', N=99 G. Table 5 (c): format 'ACO S 400 NNN', N=224 G
in source:	ClG 0043-25 = 1E 0043.3-2531
in source:	ACO 3186
in source:	ACO S 400
Ref:	=1992AJ....104.1290G
by	GARILLI B. , BOTTINI D., MACCAGNI D., VETTOLANI G., MACCACARO T.
	Astron. J., 104, 1290-1305 (1992)
	Photometric properties of three X-ray selected clusters of galaxies.
o	Table 3: <[GBM92] Cl 0043-25 A> (Nos A-H), <[GBM92] ACO 3186 A> (Nos A-H), <[GBM92] ACO S 400 A>, (Nos A-F). Table 5(a): <[GBM92] Cl 0043-25 NN> N=86. Table 5(b): <[GBM92] ACO 3186 NN> N=99. Table 5(c): <[GBM92] ACO S 400 NNN> N=224
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBM93]
[GBM93]	(Gordon+Berkermann+Mezger+, 1993)= (FIR)
Write:	<<[GBM93] FIR Na>>
N:	4
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	[GBM93] FIR 1 = NAME Sgr B2 (M). [GBM93] FIR 2 = NAME Sgr B2 (N). [GBM93] FIR 3 = NAME Sgr B2 (S)
in source:	NAME Sgr B2
Ref:	=1993A&A...280..208G
by	GORDON M.A. , BERKERMANN U., MEZGER P.G., ZYLKA R., HASLAM C.G.T., KREYSA E., SIEVERS A., LEMKE R.
	Astron. Astrophys., 280, 208-220 (1993)
	Anatomy of the Sagittarius complex. III. Morphology and characteristics of the Sgr B2 giant molecular complex.
o	<[GBM93] FIR Na> (Nos 1-3, 2a), N=4
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBN2014]
[GBN2014]	(Garcia+Bronfman+Nyman+, 2014)
Write:	<<[GBN2014] NN>> <<[GBN2014] GMC GLLL.lll+BB.bbb>>
N:	92*2
Object:	Giant MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	N=92 giant molecular clouds (GMCs) in the fourth Galactic quadrant. Use of the Columbia University - Universidad de Chile CO Survey of the southern Milky Way.
Ref:	=2014ApJS..212....2G
by	GARCIA P. , BRONFMAN L., NYMAN L.-A., DAME T.M., LUNA A.
	Astrophys. J., Suppl. Ser., 212, 2 (2014)
	Giant molecular clouds and massive star formation in the southern Milky Way.
o	Table 2: <[GBN2014] NN> (Nos 1-92) = <[GBN2014] GMC GLLL.lll+BB.bbb> N=92.
=E=	Catalogue in electronic form as <J/ApJS/212/2/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBO96]
[GBO96]	(Gallimore+Baum+O'Dea, 1996)
Write:	<<[GBO96] SN>> <<[GBO96] WW>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Comparison between HST and MERLIN image. Same map (Fig.1) as [MPH96]. The principal features are labeled as: bright central component 'C' component 'NE', component 'S' (South) with 2 subcomponents S1 and S2
in source:	NGC 1068
Ref:	=1996ApJ...458..136G
by	GALLIMORE J.F. , BAUM S.A., O'DEA C.P., PEDLAR A.
	Astrophys. J., 458, 136-148 (1996)
	The subarcsecond radio structure in NGC 1068. I. Observations and results.
o	<[GBO96] C>, <[GBO96] NE>, <[GBO96] S>, <[GBO96] SN> (Nos S1-S2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBP2017]
[GBP2017]	(Guidetti+Bondi+Prandoni+, 2017)
Write:	<<[GBP2017] JHHMMSS+DDMMSS>>
N:	94
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Jansky VLA 5.5GHz observations of N=94 radio sources in the GOODS-North field.
in source:	NAME GOODS North Field
Ref:	=2017MNRAS.471..210G
by	GUIDETTI D. , BONDI M., PRANDONI I., MUXLOW T.W.B., BESWICK R., WRIGLEY N., SMAIL I., McHARDY I., THOMSON A.P., RADCLIFFE J., ARGO M.K.
	Mon. Not. R. Astron. Soc., 471, 210-226 (2017)
	The eMERGE Survey - I: Very Large Array 5.5 GHz observations of the GOODS-North Field.
o	Table 1: <[GBP2017] JHHMMSS+DDMMSS> N=94.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBR2007]
[GBR2007]	(Gorlova+Baloo+Rieke+, 2007)
Write:	<<[GBR2007] ID NN>>
N:	13
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC, MIPS and Magellan I 6.5m telescope IMACS observations of NGC 2547. N=13 stars with excesses at 8mu.m.
in source:	NGC 2547
Ref:	=2007ApJ...670..516G
by	GORLOVA N. , BALOG Z., RIEKE G.H., MUZEROLLE J., SU K.Y.L., IVANOV V.D., YOUNG E.T.
	Astrophys. J., 670, 516-535 (2007)
	Debris disks in NGC 2547.
o	Text, figs 1, 4, Tables 4, 5: <[GBR2007] ID NN> (Nos 1-13).
=E=	Catalogue in electronic form as J/ApJ/670/516
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBR2010]
[GBR2010]	(Gratier+Braine+Rodriguez-Fernandez+, 2010)= (GMC)
Write:	<<[GBR2010] GMC NGC6822 NN>>
N:	15
Object:	Giant MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	IRAM 30-m telescope observations of NGC 6822.
in source:	NGC 6822
Ref:	=2010A&A...512A..68G
by	GRATIER P. , BRAINE J., RODRIGUEZ-FERNANDEZ N.J., ISRAEL F.P., SCHUSTER K.F., BROUILLET N., GARDAN E.
	Astron. Astrophys., 512A, 68-68 (2010)
	The molecular interstellar medium of the Local group dwarf NGC 6822. The molecular ISM of NGC 6822.
o	Table 2: <[GBR2010] GMC NGC6822 NN> (Nos 1-15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBR2012]
[GBR2012]	(GRATIER+BRAINE+RODRIGUEZ-FERNANDEZ+, 2012)
Write:	<<[GBR2012] NNN>>
N:	337
Object:	Giant MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	IRAM 30m CO(2-1) observations of M 33.
in source:	M 33
Ref:	=2012A&A...542A.108G
by	GRATIER P. , BRAINE J., RODRIGUEZ-FERNANDEZ N.J., SCHUSTER K.F., KRAMER C., CORBELLI E., COMBES F., BROUILLET N., VAN DER WERF P.P., ROELLIG M.
	Astron. Astrophys., 542A, 108-108 (2012)
	Giant molecular clouds in the Local Group galaxy M33.
o	Table A.1: <[GBR2012] NNN> (Nos 1-337).
=E=	Catalogue in electronic form as J/A+A/542/A108
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBR2017]
[GBR2017]	(Gonzalez-Lopez+Bauer+Romero-Canizales+, 2017)
Write:	<<[GBR2017] A2744-IDNN>> <<[GBR2017] MACS J0416-IDNN>> <<[GBR2017] MACS J1149-IDNN>>
N:	11+5+3
Object:	Poss. G (SIMBAD class: Galaxy_Candidate = Galaxy Candidate)
Stat:	is completely incorporated in Simbad
Note:	ALMA 1.1mm continuum observations of N=7+4+1 dusty star-forming galaxies in three galaxy clusters Abell 2744, MACS J0416.1-2403 and MACS J1149.5+2223.
in source:	ACO 2744
in source:	MCS J0416.1-2403
in source:	ClG J1149+2223
Ref:	=2017A&A...597A..41G
by	GONZALEZ-LOPEZ J. , BAUER F.E., ROMERO-CANIZALES C., KNEISSL R., VILLARD E., CARVAJAL R., KIM S., LAPORTE N., ANGUITA T., ARAVENA M., BOUWENS R.J., BRADLEY L., CARRASCO M., DEMARCO R., FORD H., IBAR E., INFANTE L., MESSIAS H., MUNOZ ARANCIBIA A.M., NAGAR N., PADILLA N., TREISTER E., TRONCOSO P., ZITRIN A.
	Astron. Astrophys., 597A, 41-41 (2017)
	The ALMA Frontier Fields Survey. I. 1.1 mm continuum detections in Abell 2744, MACS J0416.1-2403 and MACS J1149.5+2223.
o	Table 3: <[GBR2017] A2744-IDNN> (Nos ID01-ID07), <[GBR2017] MACS J0416-IDNN> (Nos ID01-ID04), <[GBR2017] MACS J1149-ID01>.
Ref:	=2018A&A...620A.125M
by	MUNOZ ARANCIBIA A.M. , GONZALEZ-LOPEZ J., IBAR E., BAUER F.E., CARRASCO M., LAPORTE N., ANGUITA T., ARAVENA M., BARRIENTOS F., BOUWENS R.J., DEMARCO R., INFANTE L., KNEISSL R., NAGAR N., PADILLA N., ROMERO-CANIZALES C., TRONCOSO P., ZITRIN A.
	Astron. Astrophys., 620A, 125-125 (2018)
	The ALMA Frontier Fields Survey. IV. Lensing-corrected 1.1 mm number counts in Abell 2744, MACS J0416.1-2403 and MACS J1149.5+2223.
o	(Erratum) erratum vol.631, art. C2 (2019)
o	Table 1 : <[GBR2017] A2744-IDNN> (Nos ID08-ID11) added, [GBR2017] MACS J0416-IDNN> (Nos ID05) added, [GBR2017] MACS J1149-IDNN> (Nos ID02-ID03) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBR99]
[GBR99]	(Georgiev+Borissova+Rosado+, 1999)
Write:	<<[GBR99] Assoc NN>> <<[GBR99] CL N>> <<[GBR99] non-stellar N>>
N:	30+2+6
Object:	Assoc. + Cl + ? (SIMBAD class: Unknown = Object of Unknown Nature)
in source:	IC 1613
Ref:	=1999A&AS..134...21G
by	GEORGIEV L. , BORISSOVA J., ROSADO M., KURTEV R., IVANOV G., KOENIGSBERGER G.
	Astron. Astrophys., Suppl. Ser., 134, 21-37 (1999)
	The Local Group dwarf irregular galaxy IC 1613. I. The young stellar content.
o	(Erratum) Erratum 1999 A&AS vol. 135, p. 197.
o	Table 6: <[GBR99] Assoc NN> (Nos 1-30). Table 7: <[GBR99] CL N> (Nos 1-2). Table 8: <[GBR99] non* N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GBS
GBS	(Galactic Bulge Survey) (Not yet in Simbad)
*****	Avoid the usage of GBS, prefer [JBN2011]
Origin	of the Acronym: L (2012ApJ...761..162H)
Details on Acronym: GBS
GBS	(Gamma Burst Source)
Write:	<<GBS HHMM+DD>>
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	Systematic designation. 1st ref.: 1982ApJ...259L..51K, N=16
Ref:	=1982ApJ...259L..51K
by	KLEBESADEL R. , EVANS W.D., LAROS J.G., STRONG I.B., CLINE T.L., DESAI U., TEEGARDEN B.J., BARAT C., HURLEY K., NIEL M., VEDRENNE G., ESTULIN I.V., KUZNETSOV A.V., ZENCHENKO V.M.
	Astrophys. J., 259, 51-56 (1982)
	A catalog of γ-ray bursts with Earth crossing times.
o	<GRB YYMMDDA> N=111, <GBS HHMM+DD> N=16
Details on Acronym: GBS
GBS	(Galactic Bulge Survey)
*****	Avoid the usage of GBS, prefer [JBN2011]
Origin	of the Acronym: L (2012ApJ...761..162H)
Details on Acronym: GBS
GBS	(Galactic Bulge Survey)
*****	Avoid the usage of GBS, prefer [JTH2014]
Origin	of the Acronym: L (2012ApJ...761..162H)
Details on Acronym: GBS-VLA
GBS-VLA	(Gould Belt Survey - Very Large Array)
Write:	<<GBS-VLA JHHMMSS.ss+DDMMSS.s>>
N:	189+146+374+206
Object:	(Radio) (SIMBAD class: Radio = Radio Source)
Note:	VLA 4 and 6cm continuum observations as part of the Gould's Belt Very Large Array Survey: N=189 sources in the Ophiuchus star-forming complex, N=146 sources in the Serpens region (Serpens molecular cloud, Serpens South cluster, W40), N=374 sources in the Orion region, N=610 sources in the Taurus-Auriga region, N=206 sources in the Perseus Region.
in source:	Gould Belt:NAME OPHIUCHUS REGION = NAME OPHIUCHUS REGION
in source:	Gould Belt:NAME SERPENS CLOUD = NAME SERPENS CLOUD
in source:	Gould Belt:NAME SERPENS SOUTH Cluster = NAME SERPENS SOUTH Cluster
in source:	Gould Belt:W 40 = W 40
in source:	Gould Belt:NAME ORI REGION = NAME ORI REGION
in source:	Gould Belt:NAME TAU-AUR REGION = NAME TAU-AUR MCLD
in source:	Gould Belt:NAME Perseus Region = NAME Perseus Region
Ref:	=2013ApJ...775...63D
by	DZIB S.A. , LOINARD L., MIODUSZEWSKI A.J., RODRIGUEZ L.F., ORTIZ-LEON G.N., PECH G., RIVERA J.L., TORRES R.M., BODEN A.F., HARTMANN L., EVANS II N.J., BRICENO C., TOBIN J.
	Astrophys. J., 775, 63 (2013)
	The Gould's Belt Very Large Array Survey. I. The Ophiuchus complex.
o	Tables 1-5: <GBS-VLA JHHMMSS.ss+DDMMSS.s> N=189.
Ref:	=2015ApJ...805....9O
by	ORTIZ-LEON G.N. , LOINARD L., MIODUSZEWSKI A.J., DZIB S.A., RODRIGUEZ L.F., PECH G., RIVERA J.L., TORRES R.M., BODEN A.F., HARTMANN L., EVANS II N.J., BRICENO C., TOBIN J., KOUNKEL M.A., GONZALEZ-LOPEZLIRA R.A.
	Astrophys. J., 805, 9 (2015)
	The Gould's Belt Very Large Array survey. II. The Serpens region.
o	Table 2: <GBS-VLA JHHMMSS.ss+DDMMSS.s> N=146.
Ref:	=2014ApJ...790...49K
by	KOUNKEL M. , HARTMANN L., LOINARD L., MIODUSZEWSKI A.J., DZIB S.A., ORTIZ-LEON G.N., RODRIGUEZ L.F., PECH G., RIVERA J.L., TORRES R.M., BODEN A.F., EVANS II N.J., BRICENO C., TOBIN J.
	Astrophys. J., 790, 49 (2014)
	The Gould's Belt Very Large Array survey. III. The Orion region.
o	Table 2: <GBS-VLA JHHMMSS.ss+DDMMSS.s> N=374.
Ref:	=2015ApJ...801...91D
by	DZIB S.A. , LOINARD L., RODRIGUEZ L.F., MIODUSZEWSKI A.J., ORTIZ-LEON G.N., KOUNKEL M.A., PECH G., RIVERA J.L., TORRES R.M., BODEN A.F., HARTMANN L., EVANS II N.J., BRICENO C., TOBIN J.
	Astrophys. J., 801, 91 (2015)
	The Gould's Belt Very Large Array survey. IV. The Taurus-Auriga complex.
o	Table 2: <GBS-VLA JHHMMSS.ss+DDMMSS.s> N=610.
Ref:	=2016ApJ...818..116P
by	PECH G. , LOINARD L., DZIB S.A., MIODUSZEWSKI A.J., RODRIGUEZ L.F., ORTIZ-LEON G.N., RIVERA J.L., TORRES R.M., BODEN A.F., HARTMAN L., KOUNKEL M.A., EVANS II N.J., BRICENO C., TOBIN J., ZAPATA L.A.
	Astrophys. J., 818, 116 (2016)
	The Gould's Belt Very Large Array Survey. V. The Perseus region.
o	Tables 2-4: <GBS-VLA JHHMMSS.ss+DDMMSS.s> N=206.
=E=	Catalogue in electronic form as <J/ApJ/775/63/>
=E=	Catalogue in electronic form as <J/ApJ/805/9/>
=E=	Catalogue in electronic form as <J/ApJ/790/49/>
=E=	Catalogue in electronic form as <J/ApJ/801/91/>
=E=	Catalogue in electronic form as <J/ApJ/818/116/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GBS2001]
[GBS2001]	(Golden+Butler+Shearer, 2001)
Write:	<<[GBS2001] NN>>
N:	39
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=39 stellar point sources within 1"05 of PSR B1821-24 position.
Ref:	=2001A&A...371..198G
by	GOLDEN A. , BUTLER R.F., SHEARER A.
	Astron. Astrophys., 371, 198-204 (2001)
	A search for the optical counterpart to PSR B1821-24 in M 28.
o	Table 1: <[GBS2001] NN> (Nos 1-39).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBS2007]
[GBS2007]	(Gardan+Braine+Schuster+, 2007)
Write:	<<[GBS2007] JHHMMSS+DDMMSS>> <<[GBS2007] JHHMMSS.s+DDMMSS>> <<[GBS2007] JHHMMSS.s+DDMMSS.s>>
N:	6
Object:	CO MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	IRAM 30m telescope CO(2-1) observations of M 33: N=6 molecular clouds are observed.
in source:	M 33 = NGC 598
Ref:	=2007A&A...473...91G
by	GARDAN E. , BRAINE J., SCHUSTER K.F., BROUILLET N., SIEVERS A.
	Astron. Astrophys., 473, 91-104 (2007)
	Particularly efficient star formation in M33.
o	Text: <[GBS2007] JHHMMSS+DDMMSS>, <[GBS2007] JHHMMSS.s+DDMMSS>, <[GBS2007] JHHMMSS.s+DDMMSS.s>, N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBS99]
[GBS99]	(Guzzo+Bohringer+Schuecker+, 1999) (Not yet in Simbad)
Write:	<<[GBS99] NN>>
N:	18
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	NAME RXC JO5169-5430
Ref:	=1999Msngr..95...27G
by	GUZZO L. , BOHRINGER H., SCHUECKER P., COLLINS C.A., SCHINDLER S., NEUMANN D.M., DE GRANDI S., CRUDDACE R., CHINCARINI G., EDGE A.C., SHAVER P.A., VOGES W.
	The Messenger, 95, 27-32 (1999)
	The REFLEX Cluster Survey: observing strategy and first results on large-scale structure.
o	Fig.4: <[GBS99] NN> (Nos 1-18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBT92]
[GBT92]	(Georgiev+Bilkina+Tikhonov, 1992)
Write:	<<[GBT92] A>> <<[GBT92] NN>> <<[GBT92] NE NN>> <<[GBT92] NW NN>> <<[GBT92] W NN>>
N:	26+89+99+44+76
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	1st ref., Table 3: format 'A' N=26, format 'NN' N=89, (Nos 1-95), (Nos 42-49) are missing. 2nd ref.: Table 4: format 'NE NN' N=99 stars in the North-Eastern area. Table 5: format 'NW NN' N=44 stars in the North-Western area. Table 6: format 'W NN' N=76 stars in the Western area. Tables 2, 3: the numberings are continuing the lists of [GTK91].
in source:	M 81 = NGC 3031
Ref:	=1992A&AS...95..581G
by	GEORGIEV T.B. , BILKINA B.I., TIKHONOV N.A.
	Astron. Astrophys., Suppl. Ser., 95, 581-588 (1992)
	The brightest blue and red stars in the galaxy M 81.
o	S = [S84b] M 81
o	Table 3: <[GBT92] A> N=26, <[GBT92] NN> N=95
Ref:	=1992A&AS...96..569G
by	GEORGIEV T.B. , BILKINA B.I., TIKHONOV N.A.
	Astron. Astrophys., Suppl. Ser., 96, 569-581 (1992)
	The distribution of blue and red stars around the M 81 galaxy.
o	Kar 952+69 = DDO 66
o	Tables 2, 3: <[GTK91] TNN> (Nos T11-T70) added, <[GTK91] NNNA> (Nos 51-110) added. Table 4: <[GBT92] NE NN> (Nos 1-99). Table 5: <[GBT92] NW NN> (Nos 1-44). Table 6: <[GBT92] W NN> (Nos 1-76).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBV2011]
[GBV2011]	(Gielen+Bouwman+van Winckel+, 2011)
Write:	<<[GBV2011] NN>>
N:	57
Object:	post-AGB* (SIMBAD class: post-AGB* = Post-AGB Star)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRS and ESO 3.6m TIMMI2 spectroscopy of N=57 post-AGB stars in the Galaxy and the LMC.
Ref:	=2011A&A...533A..99G
by	GIELEN C. , BOUWMAN J., VAN WINCKEL H., LLOYD EVANS T., WOODS P.M., KEMPER F., MARENGO M., MEIXNER M., SLOAN G.C., TIELENS A.G.G.M.
	Astron. Astrophys., 533A, 99-99 (2011)
	Silicate features in galactic and extragalactic post-AGB discs.
o	Table 1: <[GBV2011] NN> (Nos 1-33). Table 2: <[GBV2011] NN> (Nos 34-57).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GBVOC
GBVOC	(Galactic Bulge Valinhos Observatory Catalog) (Not yet in Simbad)
*****	Avoid the usage of GBVOC, prefer [TGB2011]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GBW2002]
[GBW2002]	(Gregg+Becker+White+, 2002) (Not yet in Simbad)
Write:	<<[GBW2002] J2336-0107 A>> <<[GBW2002] gN>>
N:	2+3
Object:	QSO + G (SIMBAD class: Galaxy)
Note:	For the authors SDSS J233646.20-010732.6 is a binary QSO with 2 components J2336-0107 A and B. N=3 galaxies g1 to g3 in the field of the QSOs.
Ref:	=2002ApJ...573L..85G
by	GREGG M.D. , BECKER R.H., WHITE R.L., RICHARDS G.T., CHAFFEE F.H., FAN X.
	Astrophys. J., 573, 85-89 (2002)
	An FeLoBAL binary quasar.
o	Table 1: <[GBW2002] J2336-0107 A> (Nos A-B). Fig.1: <[GBW2002] gN> (Nos g1-g3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBW2003]
[GBW2003]	(Gendre+Barret+Webb, 2003)= ([GBW2003a])
Write:	<<[GBW2003] NNN>>
N:	146
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of the globular Cluster omega Centauri, cross-correlated with Chandra observations.
in source:	Ome Cen = NGC 5139
Ref:	=2003A&A...400..521G
by	GENDRE B. , BARRET D., WEBB N.A.
	Astron. Astrophys., 400, 521-531 (2003)
	An XMM-Newton observation of the globular cluster Omega Centauri.
o	Tables 1, 2, 3: <[GBW2003] NNN> (Nos 1-146).
=E=	Catalogue in electronic form as J/A+A/400/521
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBW2003a]
[GBW2003a]	(Gendre+Barret+Webb, 2003)
*****	Avoid the usage of [GBW2003a], prefer [GBW2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBW2003b]
[GBW2003b]	(Gendre+Barret+Webb, 2003)
Write:	<<[GBW2003b] JHHMMSS.s+DDMMSS.s>>
N:	8
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of the center of the globular cluster M 13.
in source:	M 13 = NGC 6205
Ref:	=2003A&A...403L..11G
by	GENDRE B. , BARRET D., WEBB N.
	Astron. Astrophys., 403, 11-14 (2003)
	Discovery of a quiescent neutron star binary in the globular cluster M13.
o	Table 1: <[GBW2003b] JHHMMSS.s+DDMMSS.s> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBW2011]
[GBW2011]	(Ginsburg+Bally+Williams, 2011)
Write:	<<[GBW2011] NN{b\|r}>>
N:	97
Object:	Poss. Outflow (SIMBAD class: Outflow_Candidate = Outflow Candidate)
Note:	JCMT HARP CO(3-2) observations of CO outflow candidates in the W5 star forming complex.
in source:	W 5
Ref:	=2011MNRAS.418.2121G
by	GINSBURG A. , BALLY J., WILLIAMS J.P.
	Mon. Not. R. Astron. Soc., 418, 2121-2144 (2011)
	JCMT HARP CO 3–2 observations of molecular outflows in W5.
o	Tables 1+3: <[GBW2011] NNa> N=68 among (Nos 1b-40). Tables 4+5: <[GBW2011] NNa> N=29 among (Nos 41r-55r).
=E=	Catalogue in electronic form as <J/MNRAS/418/2121/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBW85]
[GBW85]	(Guilloteau+Baudry+Walmsley, 1985)
Write:	<<[GBW85] Main>> <<[GBW85] Jet>> <<[GBW85] Diffuse>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 2: Continuum sources in W 3(OH) region. See also [DW81] and [BMW93]
in source:	W 3:W 3(OH) = W 3(OH)
Ref:	=1985A&A...153..179G
by	GUILLOTEAU S. , BAUDRY A., WALMSLEY C.M.
	Astron. Astrophys., 153, 179-188 (1985)
	High resolution maps of the 2PI1/2J = 1/2OH lines in W3 (OH).
o	Table 2: <[GBW85] Main>, <[GBW85] Jet>, <[GBW85] Diffuse>, N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GBW99]
[GBW99]	(Galama+Briggs+Wijers+, 1999)
Write:	<<[GBW99] N>>
N:	8
Object:	* (SIMBAD class: Star)
Note:	Table 3: N=8 comparison stars in the field of GRB 990323.
Ref:	=1999Natur.398..394G
by	GALAMA T.J. , BRIGGS M.S., WIJERS R.A.M., VREESWIJK P.M., ROL E., BAND D., VAN PARADIJS J., KOUVELIOTOU C., PREECE R.D., BREMER M., SMITH I.A., TILANUS R.P.J., DE BRUYN A.G., STROM R.G., POOLEY G., CASTRO-TIRADO A.J., TANVIR N., ROBINSON C., HURLEY K., HEISE J., TELTING J., RUTTEN R.G.M., PACKHAM C., SWATERS R., DAVIES J.K., FASSIA A., GREEN S.F., FOSTER M.J., SAGAR R., PANDEY A.K., NILAKSHI, YADAV R.K.S., OFEK E.O., LEIBOWITZ E., IBBETSON P., RHOADS J., FALCO E., PETRY C., IMPEY C., GEBALLE T.R., BHATTACHARYA D.
	Nature, 398, 394-399 (1999)
	The effect of magnetic fields on γ-ray bursts inferred from multi-wavelength observations of the burst of 23 January 1999.
o	Table 3: <[GBW99] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GC
GC	(Green Bank obs., C list)
*****	Avoid the usage of GC, prefer [D71]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GC
GC	(General Catalog)= (B) = (BGC) = (Boss)
Write:	<<GC NNNNN>>
N:	33342
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	On magnetic tape.
Ref:	=1937GC....C......0B
by	BOSS B.
	Carnegie Institution of Washington, Publ. No 468, vol. 1-5, 0-None (1937)
	General catalogue of 33342 stars for the epoch 1950, Dudley Observatory Albany, N.Y.
o	<GC NNNNN> (Nos 1-33342).
=E=	Catalogue in electronic form as I/113
Details on Acronym: GC
GC	(Globular Cluster)
*****	Avoid the usage of GC, prefer [HJK2000]
Origin	of the Acronym: L (2007A&A...474..121B)
Details on Acronym: GC
GC	(Globular Cluster)
*****	Avoid the usage of GC, prefer [MHF2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GC
GC	(Green Bank Catalog)
*****	Avoid the usage of GC, prefer S1
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GC
GC	(Green Bank Catalog)
*****	Avoid the usage of GC, prefer S2
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GC
GC	(Green Bank Catalog)
*****	Avoid the usage of GC, prefer S3
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GC-IRAC
GC-IRAC	(Gal Center, IRAC)
*****	Avoid the usage of GC-IRAC, prefer [RAS2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GC2000]
[GC2000]	(Grebel+Chu, 2000)= (Be)
Write:	<<[GC2000] BeNN>>
N:	19
Object:	Be* (SIMBAD class: Be* = Be Star)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations.
in source:	H88 301
Ref:	=2000AJ....119..787G
by	GREBEL E.K. , CHU Y.-H.
	Astron. J., 119, 787-799 (2000)
	Hubble space telescope photometry of Hodge 301: an "old" star cluster in 30 Doradus.
o	Hodge 301 = H88 301. p.796: Shell 3 in 30 Dor = [CD83] Shell 3.
o	Table 3, col(5): <[GC2000] BeNN> (Nos Be1-Be19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GC2009]
[GC2009]	(Gruendl+Chu, 2009)
Write:	<<[GC2009] JHHMMSS.ss+DDMMSS.s>>
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Archival Spitzer IRAC and MIPS observations of the Large Magellanic Cloud. CTIO Blanco 4m telescope MOSAIC and ISPI NIR observations.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2009ApJS..184..172G
by	GRUENDL R.A. , CHU Y.-H.
	Astrophys. J., Suppl. Ser., 184, 172-197 (2009)
	High- and intermediate-mass young stellar objects in the Large Magellanic Cloud.
o	Tables 4-12: <[GC2009] JHHMMSS.ss+DDMMSS.s> N=2870.
=E=	Catalogue in electronic form as J/ApJS/184/172
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GC2020]
[GC2020]	(Gomez+Calderon, 2020)
Write:	<<[GC2020] NNN>>
N:	102
Object:	G (SIMBAD class: Galaxy)
Note:	Gemini GMOS-N spectroscopy of N= 102 galaxies in Abell 562.
in source:	ACO 562
Ref:	=2020AJ....160..152G
by	GOMEZ P.L. , CALDERON D.
	Astron. J., 160, 152-152 (2020)
	The dynamics of the wide-angle tailed (WAT) galaxy cluster A562.
o	Table 2: <[GC2020] NNN> (Nos 1-102).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GC73]
[GC73]	(Gregory+Connolly, 1973)
Write:	<<[GC73] NN>>
N:	21
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Finding chart Fig.1.
in source:	ZwCl 1609+8212
Ref:	=1973ApJ...182..351G
by	GREGORY S.A. , CONNOLLY L.P.
	Astrophys. J., 182, 351-355 (1973)
	Possible systematic redshifts in a chain of galaxies.
o	Table 1: <[GC73] NN> (Nos 1-21).
Details on Acronym: [GC94]
[GC94]	(Gavazzi+Contursi, 1994)= ([GC94a])
Write:	<<[GC94] RS NN>> <<[GC94] FG N>>
N:	92+7
Object:	(Rad) + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 2: format 'RS NN', N=92 RadioSources. Table 3: format 'FG N', N=7 Faint Galaxies.
in source:	ACO 1367
Ref:	=1994AJ....108...24G
by	GAVAZZI G. , CONTURSI A.
	Astron. J., 108, 24-32 (1994)
	Radio continuum survey of the Coma/A1367 supercluster. V. The luminosity function of A1367.
o	97064 = Z 97-6 4
o	Table 2: <[GC94] RS NN> N=92. Table 3: <[GC94] FG N> N=7
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GC94a]
[GC94a]	(Gavazzi+Contursi, 1994)
*****	Avoid the usage of [GC94a], prefer [GC94]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GC94b]
[GC94b]	(Gagne+Caillault, 1994)
Write:	<<[GC94b] NNN>>
N:	238 among 245
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Einstein observations. Somes objects missing: Nos 194, 197, 198, 199, 200, 203, 204
in source:	NAME Orion Nebula
Ref:	=1994ApJ...437..361G
by	GAGNE M. , CAILLAULT J.-P.
	Astrophys. J., 437, 361-383 (1994)
	The complete Einstein Observatory X-ray survey of the Orion nebula region.
o	<[GC94b] NNN> N=245
=E=	Catalogue in electronic form as J/ApJ/437/361
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GC98]
[GC98]	(Gorosabel+Castro-Tirado, 1998)
Write:	<<[GC98] NN>>
N:	10
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 6: N=10 objects in the error box of GRB 910122
Ref:	=1998A&A...337..691G
by	GOROSABEL J. , CASTRO-TIRADO A.J.
	Astron. Astrophys., 337, 691-698 (1998)
	Archival searches for transient optical emission in the error box of the 1991 January 22 γ-ray burst.
o	Table 6: <[GC98] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCA2018]
[GCA2018]	(Griffiths+Conselice+Alpaslan+, 2018)
Write:	<<[GCA2018] CLIO Cluster>> <<[GCA2018] NNN>> <<[GCA2018] AN.N>>
N:	1+164+4
Object:	Cluster of G + G + Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT MUSE and FORS2 observations of N=1 compact cluster, N=89 cluster members, N=75 background objects, and N=4 gravitationally lensed images.
Ref:	=2018MNRAS.475.2853G
by	GRIFFITHS A. , CONSELICE C.J., ALPASLAN M., FRYE B.L., DIEGO J.M., ZITRIN A., YAN H., MA Z., BARONE-NUGENT R., BHATAWDEKAR R., DRIVER S.P., ROBOTHAM A.S.G., WINDHORST R.A., WYITHE J.S.B.
	Mon. Not. R. Astron. Soc., 475, 2853-2869 (2018)
	MUSE spectroscopy and deep observations of a unique compact JWST target, lensing cluster CLIO.
o	<[GCA2018] CLIO Cluster> N=1. Tables 2-3: <[GCA2018] NNN> N=89+75 among (Nos 5-405). Table A1: <[GCA2018] AN.N> (Nos A1-A2, A2.1-A2.2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCB2003]
[GCB2003]	(Gavazzi+Cortese+Boselli+, 2003)
Write:	<<[GCB2003] BIG>>
N:	1
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	Loiano Cassini 1.5m telescope BFOSC and Calar Alto 2.2m telescope CAFOS observations of N=1 group of galaxies in the field of ACO 1367. In the format, BIG stands for "Blue Infalling Group".
in source:	ACO 1367
Ref:	=2003ApJ...597..210G
by	GAVAZZI G. , CORTESE L., BOSELLI A., IGLESIAS-PARAMO J., VILCHEZ J.M., CARRASCO L.
	Astrophys. J., 597, 210-217 (2003)
	Capturing a star formation burst in galaxies infalling onto the cluster A1367.
o	<[GCB2003] BIG> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCB2009]
[GCB2009]	(Gonzalez+Clowe+Bradac+, 2009)
Write:	<<[GCB2009] A>> <<[GCB2009] N>>
N:	3+7
Object:	Grav. lensed image + ? (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	Spitzer IRAC photometry of the cluster 1ES 0657-55.8 = ClG 0657-56. N=3 lensed images of a LIRG behind the cluster and N=7 objects near the images.
Ref:	=2009ApJ...691..525G
by	GONZALEZ A.H. , CLOWE D., BRADAC M., ZARITSKY D., JONES C., MARKEVITCH M.
	Astrophys. J., 691, 525-530 (2009)
	A multiply imaged luminous infrared galaxy behind the Bullet cluster (1E0657-56).
o	Fig.1, Table 1: <[GCB2009] A> (Nos A-C). Fig.1, Table 2: <[GCB2009] N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCB88]
[GCB88]	(Grabelsky+Cohen+Bronfman+, 1988)= (GMC) = (MC)
Write:	<<[GCB88] NN>> <<[GCB88] LLL.l+B.b>>
N:	43
Object:	Giant MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	Columbia CO survey of the Southern Galactic Plane. N=43 Giant Molecular Clouds in the Carina Arm. Maps in Fig.2.
in source:	NAME Carina Arm
Ref:	=1988ApJ...331..181G
by	GRABELSKY D.A. , COHEN R.S., BRONFMAN L., THADDEUS P.
	Astrophys. J., 331, 181-196 (1988)
	Molecular clouds in the Carina Arm : the largest objects; associated regions of star formation; and the Carina Arm in the Galaxy.
o	Table 2: <[GCB88] NN> (Nos 1-43) = <[GCB88] LLL.l+B.b> N=43.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCB99]
[GCB99]	(Greiner+Castro-Tirado+Boller+, 1999) (Not yet in Simbad)
Write:	<<[GCB99] A>>
N:	5
Object:	* (SIMBAD class: Star)
Note:	N=5 local standards in SAX J1810.8-2609 field.
Ref:	=1999MNRAS.308L..17G
by	GREINER J. , CASTRO-TIRADO A.J., BOLLER T., DUERBECK H.W., COVINO S., ISRAEL G.L., LINDEN-VORNLE M.J.D., OTAZU-PORTER X.
	Mon. Not. R. Astron. Soc., 308, 17-21 (1999)
	X-ray and optical-to-infrared follow-up observations of the transient X-ray burster SAX J1810.8-2609.
o	Table 3: <[GCB99] A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCC2007]
[GCC2007]	(Greco+Clementini+Catelan+, 2007)
Write:	<<[GCC2007] VNN>>
N:	29
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	Magellan Clay 6.5m telescope MagIC optical photometry of the globular cluster Fornax 4.
in source:	NAME Fornax 4
Ref:	=2007ApJ...670..332G
by	GRECO C. , CLEMENTINI G., CATELAN M., HELD E.V., PORETTI E., GULLIEUSZIK M., MAIO M., REST A., DE LEE N., SMITH H.A., PRITZL B.J.
	Astrophys. J., 670, 332-345 (2007)
	Variable stars in the Fornax dSph galaxy. I. The globular cluster Fornax 4.
o	Table 3: <[GCC2007] VNN> (Nos V1-V29).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCC2008]
[GCC2008]	(Garcia-Lorenzo+Cairos+Caon+, 2008) (Not yet in Simbad)
Write:	<<[GCC2008] Mrk NNN RN>> <<[GCC2008] III Zw 102 RN>>
N:	3+3+7+5+4
Object:	H-alpha Knot (SIMBAD class: PartofG = Part of a Galaxy)
Note:	INTEGRAL William Herschel Telescope observations.
in source:	Mrk 370
in source:	Mrk 35
in source:	Mrk 297
in source:	Mrk 314
in source:	ZW III 102
Ref:	=2008ApJ...677..201G
by	GARCIA-LORENZO B. , CAIROS L.M., CAON N., MONREAL-IBERO A., KEHRIG C.
	Astrophys. J., 677, 201-218 (2008)
	Integral field spectroscopy of blue compact dwarf galaxies.
o	Table 3: <[GCC2008] Mrk NNN RN>, <[GCC2008] III Zw 102 RN> N=3+3+7+5+4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCC2009]
[GCC2009]	(Greco+Clementini+Catelan+, 2009)
Write:	<<[GCC2009] VNN>>
N:	31
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Stat:	is completely incorporated in Simbad
Note:	6.5m Magellan Clay telescope observations of the globular cluster Fornax 5. Use of archival HST data.
in source:	NAME Fornax 5
Ref:	=2009ApJ...701.1323G
by	GRECO C. , CLEMENTINI G., CATELAN M., HELD E.V., PORETTI E., GULLIEUSZIK M., MAIO M., REST A., DE LEE N., SMITH H.A., PRITZL B.J.
	Astrophys. J., 701, 1323-1335 (2009)
	Variable stars in the Fornax dSph galaxy. III. The globular cluster Fornax 5.
o	Tables 2-4: <[GCC2009] VNN> (Nos V1-V31).
=E=	Catalogue in electronic form as <J/ApJ/701/1323/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCC2011]
[GCC2011]	(Gavazzi+Cooray+Conley+, 2011)
Write:	<<[GCC2011] GN>>
N:	5
Object:	G (SIMBAD class: Galaxy)
Note:	Keck II NIRC2 AO observations of the lensed submillimeter galaxy [CCV2011] HLSW-01.
Ref:	=2011ApJ...738..125G
by	GAVAZZI R. , COORAY A., CONLEY A., AGUIRRE J.E., AMBLARD A., AULD R., BEELEN A., BLAIN A., BLUNDELL R., BOCK J., BRADFORD C.M., BRIDGE C., BRISBIN D., BURGARELLA D., CHANIAL P., CHAPIN E., CHRISTOPHER N., CLEMENTS D.L., COX P., DJORGOVSKI S.G., DOWELL C.D., EALES S., EARLE L., ELLSWORTH-BOWERS T.P., FARRAH D., FRANCESCHINI A., FU H., GLENN J., GONZALEZ SOLARES E.A., GRIFFIN M., GURWELL M.A., HALPERN M., IBAR E., IVISON R.J., JARVIS M., KAMENETZKY J., KIM S., KRIPS M., LEVENSON L., LUPU R., MAHABAL A., MALONEY P.D., MARASTON C., MARCHETTI L., MARSDEN G., MATSUHARA H., MORTIER A.M.J., MURPHY E., NAYLOR B.J., NERI R., NGUYEN H.T., OLIVER S.J., OMONT A., PAGE M.J., PAPAGEORGIOU A., PEARSON C.P., PEREZ-FOURNON I., POHLEN M., RANGWALA N., RAWLINGS J.I., RAYMOND G., RIECHERS D., RODIGHIERO G., ROSEBOOM I.G., ROWAN-ROBINSON M., SCHULZ B., SCOTT D., SCOTT K.S., SERRA P., SEYMOUR N., SHUPE D.L., SMITH A.J., SYMEONIDIS M., TUGWELL K.E., VACCARI M., VALIANTE E., VALTCHANOV I., VERMA A., VIEIRA J.D., VIGROUX L., WANG L., WARDLOW J., WIEBE D., WRIGHT G., XU C.K., ZEIMANN G., ZEMCOV M., ZMUIDZINAS J.
	Astrophys. J., 738, 125 (2011)
	Modeling of the HerMES submillimeter source lensed by a dark matter dominated foreground group of galaxies.
o	Fig. 1: <[GCC2011] GN> (Nos G1-G5), <[CCV2011] HLSW-01 Na> (Nos 1a-1b) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCC2013]
[GCC2013]	(Garofalo+Cusano+Clementini +, 2013)
Write:	<<[GCC2013] VN>>
N:	7 (SIMBAD class: RRLyrae = RR Lyrae Variable)
Note:	Cassini Telescope, Thueringer Landessternwarte Tautenburg Telescope and Toppo telescope observations of N=7 RR Lyrae Stars in Ursa Major.
in source:	NAME UMa I Galaxy
Ref:	=2013ApJ...767...62G
by	GAROFALO A. , CUSANO F., CLEMENTINI G., RIPEPI V., DALL'ORA M., MORETTI M.I., COPPOLA G., MUSELLA I., MARCONI M.
	Astrophys. J., 767, 62 (2013)
	Variable stars in the ultra-faint dwarf spheroidal galaxy Ursa Major I.
o	Table 2: <[GCC2013] VN> (Nos V1 to V7).
=E=	Catalogue in electronic form as <J/ApJ/767/62/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCC95]
[GCC95]	(Gavazzi+Contursi+Carrasco+, 1995) (Not yet in Simbad)
Write:	<<[GCC95] Z 97-73 A>> <<[GCC95] Z 97-79 A>>
N:	4+5
Object:	HII (SIMBAD class: HIIReg = HII Region)
in source:	Z 97-73
in source:	Z 97-79
Ref:	=1995A&A...304..325G
by	GAVAZZI G. , CONTURSI A., CARRASCO L., BOSELLI A., KENNICUTT R., SCODEGGIO M., JAFFE W.
	Astron. Astrophys., 304, 325-340 (1995)
	The radio and optical structure of three peculiar galaxies in A 1367.
o	Table 4, Fig.2a: <[GCC95] Z 97-73 A> (Nos A-D). Table 4, Fig.2b: <[GCC95] Z 97-79 A> (Nos A-E). Table 4, Fig.2c: <[GTJ84] AN> (No. B3) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCC96]
[GCC96]	(Graham+Clowes+Campusano, 1996)
Write:	<<[GCC96] HHMM+DDMM>>
N:	1
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Ref:	=1996MNRAS.279.1349G
by	GRAHAM M.J. , CLOWES R.G., CAMPUSANO L.E.
	Mon. Not. R. Astron. Soc., 279, 1349-1356 (1996)
	A quasar with ultrastrong, ultraviolet Fe II emission.
o	<[GCC96] 2226-3905> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCC98]
[GCC98]	(Ganguly+Churchill+Charlton, 1998) (Not yet in Simbad)
Write:	<<[GCC98] Cloud A>>
N:	2
Object:	Cloud (SIMBAD class: Cloud)
Note:	In the spectrum of the QSO 1222+228, the authors found N=2 absorbing clouds.
Ref:	=1998ApJ...498L.103G
by	GANGULY R. , CHURCHILL C.W., CHARLTON J.C.
	Astrophys. J., 498, 103-106 (1998)
	An aluminum-enhanced cloud in a C IV absorber at z = 1.94.
o	Table 1: <[GCC98] Cloud A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GCCCS
GCCCS	(General Catalog of Cool Carbon *)
**	catalog: use C*
Origin	of the Acronym: L = Found in the literature
Details on Acronym: GCCGCS
GCCGCS	(General Catalog of Cool Gal. Carbon *)
**	catalog: use CGCS
Origin	of the Acronym: L = Found in the literature
Details on Acronym: GCCR
GCCR	(Galactic Center Compact Radio) (Not yet in Simbad)
*****	Avoid the usage of GCCR, prefer [ZMG2020]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GCCS
GCCS	(General Catalog of Carbon *)
**	catalog: use C*
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GCD95]
[GCD95]	(Gaume+Claussen+De Pree+, 1995)= (Sgr)
Write:	<<[GCD95] ASS.sss>>
N:	24
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	The authors used a new format which combine the old format used in [BJ84] with a new naming scheme: format ' ASS.sss', the letter 'A' as the same convention as the previous lettering, and 'SS.sss' are the seconds of right ascension of the source. For ex.: a newly detected component near the Sgr B2 F region ([BJ84] F) having a right ascension of 17h44m10.27 would have a format of 'F10.27'. See [BJ84]
in source:	NAME Sgr B2
Ref:	=1995ApJ...449..663G
by	GAUME R.A. , CLAUSSEN M.J., DE PREE C.G., GOSS W.M., MEHRINGER D.M.
	Astrophys. J., 449, 663-673 (1995)
	The Sagittarius B2 star-forming region. I. Sensitive 1.3 centimeter continuum observations.
o	Table 2: <[BJ84] K6> N=1 added. Table 2: <[GCD95] ASS.ss> N=23
Ref:	=1998ApJ...500..847D
by	DE PREE C.G. , GOSS W.M., GAUME R.A.
	Astrophys. J., 500, 847-852 (1998)
	Ionized gas in Sagittarius B2 main on scales of 0.065 arcsecond (600 AU).
o	Table 1: <[GCD95] F10.38> N=1 added. Table 1: <[BJ84] FNa> (Nos F1a-F1g, F2a-F2d, F3a-F3e, F4a-F4c).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCD96]
[GCD96]	(Giallongo+Cristiani+D'Odorico+, 1996)
Write:	<<[GCD96] HHMM+DD>>
N:	10
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Ref:	=1996ApJ...466...46G
by	GIALLONGO E. , CRISTIANI S., D'ODORICO S., FONTANA A., SAVAGLIO S.
	Astrophys. J., 466, 46-54 (1996)
	The proximity effect, the UV background, and the statistics of the Lyα lines at high resolution.
o	Table 1: <[GCD96] HHMM+DD> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCE2020]
[GCE2020]	(Gregory+Collins+Erkal+, 2020)
Write:	<<[GCE2020] NNN>>
N:	21
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Keck II DEIMOS spectroscopy of N=21 members of the Hercules dwarf galaxy.
in source:	NAME Hercules Dwarf Galaxy
Ref:	=2020MNRAS.496.1092G
by	GREGORY A.L. , COLLINS M.L.M., ERKAL D., TOLLERUD E., DELORME M., HILL L., SAND D.J., STRADER J., WILLMAN B.
	Mon. Not. R. Astron. Soc., 496, 1092-1104 (2020)
	Uncovering the orbit of the hercules dwarf galaxy.
o	Table 2: <[GCE2020] NNN> N=21 among (Nos 2-117).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCF2002]
[GCF2002]	(Gandhi+Crawford+Fabian, 2002)
Write:	<<[GCF2002] MS 2137-N>> <<[GCF2002] A 1835-NW>> <<[GCF2002] A 2204-N>>
N:	4+4+2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra X-ray sources in 3 ClG, and components. Maps in Fig.4. See also [CFG2001b] and [CGF2002].
in source:	1E 2137.0-2353
in source:	ACO 1835
in source:	ACO 2204
Ref:	=2002MNRAS.337..781G
by	GANDHI P. , CRAWFORD C.S., FABIAN A.C.
	Mon. Not. R. Astron. Soc., 337, 781-794 (2002)
	Very Large Telescope near-infrared spectra of hard serendipitous Chandra sources.
o	Table 1: <[GCF2002] MS 2137-N> (Nos 1 to 4), <[GCF2002] A 1835-NW> (Nos 1, 2, 1E, 1W), <[GCF2002] A 2204-N> (Nos 1, 2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCF2004]
[GCF2004]	(Gandhi+Crawford+Fabian+, 2004)
Write:	<<[GCF2004] Per N>> <<[GCF2004] RX J0820.9+0752 N>> <<[GCF2004] B2 0902+34 N>> <<[GCF2004] IRAS 09104+4109 N>> <<[GCF2004] ACO NNNN NN>> <<[GCF2004] 3C 294 N>> <<[GCF2004] MS 2137.3-2353 N>>
N:	64
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Small sample of Chandra X-ray sources selected from 12 fields of ACIS observations.
Ref:	=2004MNRAS.348..529G
by	GANDHI P. , CRAWFORD C.S., FABIAN A.C., JOHNSTONE R.M.
	Mon. Not. R. Astron. Soc., 348, 529-550 (2004)
	Powerful, obscured active galactic nuclei among X-ray hard, optically dim serendipitous Chandra sources.
o	Table 3: <[GCF2004] Per N> (No. 2), <[GCF2004] RX J0820.9+0752 N> (Nos 1-4), <[GCF2004] B2 0902+34 N> (No. 1), <[GCF2004] IRAS 09104+4109 N> (Nos 1-3), <[GCF2004] ACO NNNN N> N=14+2+4+8+2+17, <[GCF2004] 3C 294 N> (Nos 1-3), <[GCF2004] MS 2137.3-2353 N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCF2012]
[GCF2012]	(Grazian+Castellano+Fontana+, 2012)
Write:	<<[GCF2012] GDS NNNNN>> <<[GCF2012] P12HUDF NNNN>> <<[GCF2012] UDS NNNNN>> <<[GCF2012] EGS NNNNN>>
N:	21+23+46+21
Object:	G (SIMBAD class: Galaxy)
Note:	N=21+23+46+21 z∼7 galaxy candidates in the GOODS-South Deep field (GDS), the HUDF P12 field, the Ultra Deep survey field (UDS) and the Extended Groth Strip survey field (EGS). Use of CANDELS Deep+Wide surveys, as well as data from the HUDF09 program.
Ref:	=2012A&A...547A..51G
by	GRAZIAN A. , CASTELLANO M., FONTANA A., PENTERICCI L., DUNLOP J.S., McLURE R.J., KOEKEMOER A.M., DICKINSON M.E., FABER S.M., FERGUSON H.C., GALAMETZ A., GIAVALISCO M., GROGIN N.A., HATHI N.P., KOCEVSKI D.D., LAI K., NEWMAN J.A., VANZELLA E.
	Astron. Astrophys., 547A, 51-51 (2012)
	The size-luminosity relation at z=7 in CANDELS and its implication on reionization.
o	Table A.1: <[GCF2012] GDS NNNNN> N=21 among (Nos 565-13233). Table A.2: <[GCF2012] P12HUDF NNNN> N=23 among (Nos 173-2261). Table A.3: <[GCF2012] UDS NNNNN> N=46 among (Nos 2047-34364). Table A.4: <[GCF2012] EGS NNNNN> N=21 among (Nos 1976-21147).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCF93]
[GCF93]	(Galli+Cappi+Focardi+, 1993)
Write:	<<[GCF93] ACO NNNN NN>>
N:	65
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	In the format 'ACO NNNN' stands for 13 ACO Clusters, 'NN' a running number for galaxies in each cluster. Tables 1 and 2: ACO 3111: N=5, AC0 3135: N=5, ACO 3354: N=1, ACO 3390: N=11, ACO 3392: N=5, ACO 3407: N=3, ACO 2799: N=4, ACO 2911: N=10, ACO 3094: N=4, ACO 3122: N=3, ACO 3151: N=3, ACO 3223: N=4, ACO 3341: N=7. Finding charts. See also [VCC89], [CFG91] G in ACO 2799, 2911, 3094, 3122, 3223 and 3341 complete [CFG91].
in source:	ACO 3111
in source:	ACO 3135
in source:	ACO 3354
in source:	ACO 3390
in source:	ACO 3392
in source:	ACO 3407
in source:	ACO 2799
in source:	ACO 2911
in source:	ACO 3094
in source:	ACO 3122
in source:	ACO 3151
in source:	ACO 3223
in source:	ACO 3341
Ref:	=1993A&AS..101..259G
by	GALLI M. , CAPPI A., FOCARDI P., GREGORINI L., VETTOLANI G.
	Astron. Astrophys., Suppl. Ser., 101, 259-265 (1993)
	Redshifts of southern rich clusters.
o	Tables 1, 2: <[GCF93] ACO NNNN NN> N=65
=E=	Catalogue in electronic form as J/A+AS/101/259
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCG2013]
[GCG2013]	(Grillo+Christensen+Gallazzi+, 2013)
Write:	<<[GCG2013] BG>> <<[GCG2013] GN>> <<[GCG2013] aN>>
N:	5+5
Object:	Grav. lensed image + Grav. lens (SIMBAD class: GravLens = Gravitational Lens)
Note:	VLT X-Shooter of N=5 lens massive galaxies and N=5 lensed images. Use of Gemini Science Archive and SDSS data.
in source:	CSWA 31
Ref:	=2013MNRAS.433.2604G
by	GRILLO C. , CHRISTENSEN L., GALLAZZI A., RASMUSSEN J.
	Mon. Not. R. Astron. Soc., 433, 2604-2612 (2013)
	Measuring the total and baryonic mass profiles of the very massive CASSOWARY 31 strong lens. A fossil system at z ≃ 0.7 ?
o	Table 1: <[GCG2013] BG>, <[GCG2013] GN> (Nos G1-G4), <[GCG2013] aN> (Nos i1-i4, j1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GCGSS
GCGSS	(General Catalog of Gal. S Stars)
**	catalog: use CSS
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GCH2001]
[GCH2001]	(Gallagher+Charlton+Sally+, 2001)
Write:	<<[GCH2001] NNN>>
N:	139
Object:	Poss. Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST WFPC2 search for candidate star clusters in the Stephan's Quintet.
in source:	Stephan's Quintet = HCG 92
Ref:	=2001AJ....122..163G
by	GALLAGHER S.C. , CHARLTON J.C., HUNSBERGER S.D., ZARITSKY D., WHITMORE B.C.
	Astron. J., 122, 163-181 (2001)
	Hubble space telescope images of Stephan's quintet: star cluster formation in a compact group environment.
o	Tables 1-4: <[GCH2001] NNN> (Nos 1-139).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCH2007]
[GCH2007]	(Gronwall+Ciardullo+Hickey+, 2007)= (LAE)
Write:	<<[GCH2007] NNN>>
N:	259
Object:	LAE G (SIMBAD class: EmObj = Emission Object)
Note:	MOSAIC II CCD camera on the CTIO Blanco 4m telescope observations of the CDFS.
in source:	NAME CDFS
Ref:	=2007ApJ...667...79G
by	GRONWALL C. , CIARDULLO R., HICKEY T., GAWISER E., FELDMEIER J.J., VAN DOKKUM P.G., URRY C.M., HERRERA D., LEHMER B.D., INFANTE L., ORSI A., MARCHESINI D., BLANC G.A., FRANCKE H., LIRA P., TREISTER E.
	Astrophys. J., 667, 79-91 (2007)
	Lyα emission-line galaxies at z = 3.1 in the Extended Chandra Deep Field-South.
o	Tables 2, 3: <[GCH2007] NNN> (Nos 1-259).
=E=	Catalogue in electronic form as J/ApJ/667/79
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCH2011]
[GCH2011]	(Gotz+Covino+Hascoet+, 2011)
Write:	<<[GCH2011] J002427.6+625033.5>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	CFHT observations of the host galaxy of GRB 041219A.
Ref:	=2011MNRAS.413.2173G
by	GOTZ D. , COVINO S., HASCOET R., FERNANDEZ-SOTO A., DAIGNE F., MOCHKOVITCH R., ESPOSITO P.
	Mon. Not. R. Astron. Soc., 413, 2173-2183 (2011)
	A detailed spectral study of GRB 041219A and its host galaxy.
o	Table 2: <[GCH2011] J002427.6+625033.5> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GCIRS
GCIRS	(Gal. Center, IR Source)= (BN) = (IRS) = (RL)
Write:	<<GCIRS NN>> <<GCIRS NNA>> <<GCIRS NNAA>> <<GCIRS NNW>> <<GCIRS NNWA>> <<GCIRS NNWN>> <<GCIRS NNWNa>> <<GCIRS NNWNW>> <<GCIRS NNWW>> <<GCIRS NNWWN>> <<GCIRS NNWWW>> <<GCIRS NNWWWN>> <<GCIRS NN>> <<GCIRS* NNWext>> <<GCIRS NNWWext>> <<GCIRS 16UN>> <<GCIRS ANN>>
N:	144
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	N=36 IR sources, (Nos 1-36) and their components. Later, N=24 new sources 'ANN' (Nos A1-A24)
in source:	NAME Gal Center
Ref:	=1973ApJ...184..415R
by	RIEKE G.H. , LOW F.J.
	Astrophys. J., 184, 415-425 (1973)
	Infrared maps of the Galactic Nucleus.
o	Table 2: <GCIRS N> (Nos 1-5)
Ref:	=1975ApJ...200L..71B
by	BECKLIN E.E. , NEUGEBAUER G.
	Astrophys. J., 200, 71-74 (1975)
	High resolution maps of the Galactic Center at 2.2 and 10 microns.
o	Table 1: <GCIRS NN> (Nos 6-19) added.
Ref:	=1978ApJ...219..121B
by	BECKLIN E.E. , MATTHEWS K., NEUGEBAUER G., WILLNER S.P.
	Astrophys. J., 219, 121-128 (1978)
	Infrared observations of the Galactic Center. I. Nature of the compact sources.
o	<GCIRS NN> (No. 20) added.
Ref:	=1978ApJ...220..556R
by	RIEKE G.H. , TELESCO C.M., HARPER D.A.
	Astrophys. J., 220, 556-567 (1978)
	The infrared emission of the Galactic Center.
o	The SW source in table 1 is the IRS No. 21 in Gal Center (1982ApJ...263..672L)
o	Table 1: <GCIRS NN> No. 21 is new
Ref:	=1979AJ.....84..324L
by	LEBOFSKY M.J.
	Astron. J., 84, 324-328 (1979)
	Variable extinction at the Galactic Center.
o	<GCIRS NN> (No. 22) added.
Ref:	=1982ApJ...263..672L
by	LEBOFSKY M.J. , RIEKE G.H., DESHPANDE M.R., KEMP J.C.
	Astrophys. J., 263, 672-676 (1982)
	Polarization of compact sources in the Galactic Center.
o	Table 2: <GCIRS NN> (Nos 22-27) are new
Ref:	=1983MNRAS.204.1153S
by	STOREY J.W.V. , ALLEN D.A.
	Mon. Not. R. Astron. Soc., 204, 1153-1161 (1983)
	The galactic nucleus.
o	Fig 1: object NIR 3 not in SIMBAD. Table 1: [SSJ82] Star A and B, [SSJ82] CCD 1 and 2.
o	Table 1: <GCIRS NNWW> (Nos 1W, 1E, 16NE, 16SE), <GCIRS NNA> No. 16C
Ref:	=1986ApJ...301L..49F
by	FORREST W.J. , PIPHER J.L., STEIN W.A.
	Astrophys. J., 301, 49-52 (1986)
	Sagittarius A and the positions of infrared sources in the Galactic Center.
o	Table 1: <GCIRS NNWW> (No. 16NW) added.
Ref:	=1988ApJ...327L..65A
by	ADAMS D.J. , BECKLIN E.E., JAMESON R.F., LONGMORE A.J., SANDQVIST A., VALENTIJN E.
	Astrophys. J., 327, 65-68 (1988)
	Lunar occultation of the Galactic Center at 2.2 microns.
o	Table 1: <GCIRS 16UN> (Nos 16U1-16U3)
Ref:	=1989ApJ...336..752R
by	RIEKE G.H. , RIEKE M.J., PAUL A.E.
	Astrophys. J., 336, 752-761 (1989)
	Origin of the excitation of the Galactic Center.
o	Table 1, Fig. 1: <GCIRS NNWW> (Nos 1NE, 1SE, 10E, 10W, 15E, 15W) are new
Ref:	=1989AJ.....98..204T
by	TOLLESTRUP E.V. , CAPPS R.W., BECKLIN E.E.
	Astron. J., 98, 204-216 (1989)
	High-resolution IRCCD images of the Galactic Center at 2.2 and 3.5 microns.
o	Tables I, II: <GCIRS NNWWW> (Nos 2E, 6E, 6W, 12N, 12S, 14NE, 14SW, 16SWE, 16SWW, 16SWS) and (Nos 28-32) are new
Ref:	=1990ApJ...360...95S
by	SIMON M. , CHEN W.P., FORREST W.J., GARNETT J.D., LONGMORE A.J., GAUER T., DIXON R.I.
	Astrophys. J., 360, 95-105 (1990)
	Subarcsecond resolution observations of the central parsec of the galaxy at 2.2 microns.
o	Table 2, Fig. 1: <GCIRS NNWW> (Nos 1WW, 1WE, 2S, 7SE, 13E, 13W) and (Nos 33-36), <GCIRS NNWWext> No. 16SWext
Ref:	=1991AJ....101.1324D
by	DEPOY D.L. , SHARP N.A.
	Astron. J., 101, 1324-1328 (1991)
	High resolution infrared imaging of the Galactic Center.
o	Table 1, Fig 5: <GCIRS NNW> No. 16S, <GCIRS NNAA> No. 16CC, <GCIRS NNWext> No. 16Sext, are new
Ref:	=1991ApJ...382L..19K
by	KRABBE A. , GENZEL R., DRAPATZ S., ROTACIUC V.
	Astrophys. J., 382, 19-22 (1991)
	A cluster of He I emission-line stars in the Galactic Center.
o	<[KGD91] HeI Cluster> N=1. Table 1: <[KGD91] HeI NN> (Nos 1-17). Table 1: <GCIRS NNWW> (Nos 7W, 11S, 15NE, 15SW) added.
Ref:	=1992A&A...257..515R
by	ROSA M.R. , ZINNECKER H., MONETI A., MELNICK J.
	Astron. Astrophys., 257, 515-522 (1992)
	The Galactic Center in the Far-Red.
o	Table 3: <GCIRS NNA> No. 12C is new, <GZ A> (Nos A-B)
Ref:	=1993AJ....105..956H
by	HERBST T.M. , BECKWITH S.V.W., FORREST W.J., PIPHER J.L.
	Astron. J., 105, 956-970 (1993)
	Infrared imaging spectroscopy of the galactic center: distribution and motions of the ionized gas.
o	Fig. 1: <GCIRS NNW> (No. 1SW) added.
Ref:	=1996ApJ...467..645T
by	TAMURA M. , WERNER M.W., BECKLIN E.E., PHINNEY E.S.
	Astrophys. J., 467, 645-657 (1996)
	Detection of stellar variability in the central parsec of the Galaxy.
o	Table 1: <GCIRS NN> No. 10 is new, <GCIRS ANN> (Nos A1-A24)
Ref:	=1996Natur.383..415E
by	ECKART A. , GENZEL R.
	Nature, 383, 415-417 (1996)
	Observations of stellar proper motions near the Galactic Centre.
o	Table 1: only GCIRS and BHA sources are in SIMBAD.
o	Table 1: <GCIRS NNWWN> (Nos 16SE1, 16SE2, 29N, 29S, 33E, 33W, 34W) are new. <BHA NW> (Nos 4E, 4W)
Ref:	=1996ApJ...470..864B
by	BLUM R.D. , SELLGREN K., DEPOY D.L.
	Astrophys. J., 470, 864-881 (1996)
	JHKL photometry and the K-band luminosity function at the Galactic Center.
o	T.1, cross-id. col(2): GCIRS, MPE, OSU, Tam, NAME BSD WC9, NAME AF star, NAME AF NW, NAME AF NWB, F95 A, B, j From Figer Thesis, not in SIMBAD
o	Table 1: <[BSD96] NNN> (Nos 1-147), <GCIRS NNWA>, <GCIRS NNA> (Nos 2L, 6WB, 10EL, 12NB, 30B). <NAME AF NWB>. Table 1, col(2): <OSU CN> (Nos C1-C4), <OSU F1>, <OSU He1>
Ref:	=1997A&A...325..700N
by	NAJARRO F. , KRABBE A., GENZEL R., LUTZ D., KUDRITZKI R.P., HILLIER D.J.
	Astron. Astrophys., 325, 700-708 (1997)
	Quantitative spectroscopy of the HeI cluster in the Galactic Center.
o	<GCIRS NNWN> No. 13E1
Ref:	=1997MNRAS.291..219G
by	GENZEL R. , ECKART A., OTT T., EISENHAUER F.
	Mon. Not. R. Astron. Soc., 291, 219-234 (1997)
	On the nature of the dark mass in the centre of the Milky Way.
o	Table 1: sources S1 to S11 = [EG97] SNN
o	Fig.1: <[EG97] S12> added. Table 1: <GCIRS 29S1>, <GCIRS 29S2> new. Table 1: <[GEO97] WNN> (Nos W1-W18).
Ref:	=1999ApJ...523..248O
by	OTT T. , ECKART A., GENZEL R.
	Astrophys. J., 523, 248-264 (1999)
	Variable and embedded stars in the galactic center.
o	Table 2: <[OEG99] NNN> (Nos 1-218). Table 2: <GCIRS NNWW> N=7 new. Table 2: <MPE +x.x+yy.y> N=10 new.
Ref:	=2000MNRAS.317..348G
by	GENZEL R. , PICHON C., ECKART A., GERHARD O.E., OTT T.
	Mon. Not. R. Astron. Soc., 317, 348-374 (2000)
	Stellar dynamics in the Galactic Centre: proper motions and anisotropy.
o	Table 1, col(19): w217 ?? ID not identified (= [GPE2000] 1.34)
o	Table 1, col(1): <[GPE2000] NN.NNA> N=299. Table 1, col(19): <GCIRS NWWN> N=6 added. Table 1, col(19): <[EG97] SNN> (Nos S18-S19) added.
Ref:	=2004ApJ...602..760E
by	ECKART A. , MOULTAKA J., VIEHMANN T., STRAUBMEIER C., MOUAWAD N.
	Astrophys. J., 602, 760-769 (2004)
	Young stars at the center of the Milky way.
o	Table 2: <[EMV2004] aaa> N=8. Table 2: <GCIRS NNWNa> (No. 13E3c>, <GCIRS NNWNW> (No. 13E3N>.
Ref:	=2008A&A...478..127P
by	PERGER M. , MOULTAKA J., ECKART A., VIEHMANN T., SCHOEDEL R., MUZIC K.
	Astron. Astrophys., 478, 127-135 (2008)
	Compact mid-IR sources east of Galactic Center source IRS 5.
o	Table 1, Fig.3: <GCIRS 5WN>, <GCIRS 5WWN> N=9 added. Table 1, Fig.4: <[PME2008] NNa> (Nos 1-13, 14a-14e, 15-20, 21a-21c).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GCK
GCK	(GALEX-CAUSE Kepler Survey)
Write:	<<GCK JHHMMSSss+DDMMSSs>>
N:	660928
Object:	(NUV) (SIMBAD class: UV = UV-emission Source)
Note:	Deep near-ultraviolet (NUV) photometric survey of the Kepler field with the Galaxy Evolution Explorer (GALEX) Complete All-Sky UV Survey Extension (CAUSE). The GALEX-CAUSE Kepler survey (GCK) covers 104 square degrees of the Kepler field and reaches a limiting magnitude of NUV∼22.6 at 3σ.
Ref:	=2015ApJ...813..100O
by	OLMEDO M. , LLOYD J., MAMAJEK E.E., CHAVEZ M., BERTONE E., MARTIN D.C., NEILL J.D.
	Astrophys. J., 813, 100 (2015)
	Deep GALEX UV survey of the Kepler field. I. Point source catalog.
o	Table 4: <GCK JHHMMSSss+DDMMSSs> N=660928.
=E=	Catalogue in electronic form as J/ApJ/813/100
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GCK2014]
[GCK2014]	(Gvaramadze+Chene+Kniazev+, 2014)= (BAT99) (Not yet in Simbad)
Write:	<<[GCK2014] BAT99 Na>>
N:	1
Object:	WR* (SIMBAD class: WolfRayet* = Wolf-Rayet)
Note:	Gemini South GMOS spectroscopic observations of N=1 Wolf-Rayet star in the LMC.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2014MNRAS.442..929G
by	GVARAMADZE V.V. , CHENE A.-N., KNIAZEV A.Y., SCHNURR O., SHENAR T., SANDER A., HAINICH R., LANGER N., HAMANN W.-R., CHU Y.-H., GRUENDL R.A.
	Mon. Not. R. Astron. Soc., 442, 929-945 (2014)
	Discovery of a new Wolf-Rayet star and a candidate star cluster in the Large Magellanic Cloud with Spitzer.
o	Table 1: <[GCK2014] BAT99 Na> (No 3a).
o	star 1 = IRSF J04530376-6923518, star 2 = IRSF J04530360-6923538, star 3 = IRSF J04530386-6923509.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCK99]
[GCK99]	(Garcia-Barreto+Combes+Koribalski+, 1999)
Write:	<<[GCK99] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=1 small galaxy NW of NGC 3783.
Ref:	=1999A&A...348..685G
by	GARCIA-BARRETO J.A. , COMBES F., KORIBALSKI B., FRANCO J.
	Astron. Astrophys., 348, 685-692 (1999)
	HI spatial distribution in the galaxy NGC 3783.
o	p. 689: <[GCK99] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GCl
GCl	(Globular Cluster)
Write:	<<GCl NNN>> <<GCl NNN.N>>
N:	137
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Ref:	=1970CSCA..C......0A
by	ALTER G. , RUPRECHT J., VANYSEK V.
	Catalogue of star clusters and associations + supplements. Akad. Kiado, Budapest, Hungary, 3086 p., 2nd edition,1970, 0-None (1970)
	Catalogue of star clusters and associations + supplements.
o	<Assoc NN.N>. <GCl NNN.N>. <OCl NNNN.N>.
Ref:	=1981CSCAS.C......0R
by	RUPRECHT J. , BALAZS B., WHITE R.E.
	Akad. Kiado, Budapest, Hungary,1981, 0-None (1981)
	Catalogue of star clusters and associations. Suppl. 1 to the 2nd edition.
o	<Assoc NN.N> (Nos 1-70), N=89. <GCl NNN.N> (Nos 1-125), N=137. <OCl NNNN.N> (Nos 1-1044) N=1112.
=E=	Catalogue in electronic form as VII/44
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GCL88]
[GCL88]	(Garcia+Claria+Levato, 1988)
Write:	<<[GCL88] NNN>>
N:	90 among 478
Object:	* in Assoc. (SIMBAD class: Star)
in source:	NAME ASS CAR OB 2-
Ref:	=1988Ap&SS.143..317G
by	GARCIA B. , CLARIA J.J., LEVATO H.
	Astrophys. Space Sci., 143, 317-328 (1988)
	The ratio of total to selective absorption in the Carina OB2 association.
o	Table I: 2330 misprint for 233
o	Table I: <[GCL88] NNN> N=90 among 478
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCL96]
[GCL96]	(Garnavich+Challis+Leibundgut+, 1996)
Write:	<<[GCL96] JHHMMSS.ss+DDMMSS.s>>
N:	7
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxies of SN 1996E to SN 1996K.
Ref:	=1996IAUC.6332Q...1G
by	GARNAVICH P. , CHALLIS P., LEIBUNDGUT B., SUNTZEFF N., CLOCCHIATTI A., SCHMIDT B., TURNER E., ATHEY A.
	IAU Circ., 6332, 1-None (1996)
	Supernovae.
o	<[GCL96] JHHMMSS.ss+DDMMSS.s> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GCM
GCM	(Gal. Center Molecular cloud)= (M) = (MC)
Write:	<<GCM +LL.ll+BB.bb>> <<GCM +LL.lll+BB.bbb>>
N:	88
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
in source:	NAME Gal Center
Ref:	=1981A&A...103..197G
by	GUSTEN R. , WALMSLEY C.M., PAULS T.
	Astron. Astrophys., 103, 197-206 (1981)
	Ammonia in the neighbourhood of the Galactic Center.
o	<GCM +LL.ll+BB.bb> N=7.
Ref:	=1985A&A...142..381G
by	GUSTEN R. , WALMSLEY C.M., UNGERECHTS H., CHURCHWELL E.
	Astron. Astrophys., 142, 381-387 (1985)
	Temperature determinations in molecular clouds of the Galactic Center.
o	Table 1: <GCM +LL.ll+BB.bb> N=4 added.
Ref:	=1987A&A...184..133S
by	SERABYN E. , GUSTEN R.
	Astron. Astrophys., 184, 133-143 (1987)
	A molecular counterpart to the Galactic Center Arc.
o	Molecular cloud later designated as <GCM +0.10+0.03>
Ref:	=1994ApJ...424L..91S
by	SERABYN E. , MORRIS M.
	Astrophys. J., 424, 91-94 (1994)
	The source of the relativistic particles in the Galactic Center Arc.
o	<GCM +LL.ll+BB.bb> N=2.
Ref:	=1993A&A...280..255H
by	HUETTEMEISTER S. , WILSON T.L., BANIA T.M., MARTIN-PINTADO J.
	Astron. Astrophys., 280, 255-267 (1993)
	Kinetic temperatures in Galactic Center molecular clouds.
o	<GCM +LL.ll+BB.bb> N=34.
Ref:	=1995A&A...298..473U
by	UCHIDA K.I. , GUESTEN R.
	Astron. Astrophys., 298, 473-481 (1995)
	The large-scale magnetic field in the Galactic Center.
o	Table 1: <GCM +.ll+B.bb> N=13
Ref:	=2001A&A...365..174R
by	RODRIGUEZ-FERNANDEZ N.J. , MARTIN-PINTADO J., FUENTE A., DE VICENTE P., WILSON T.L., HUETTEMEISTER S.
	Astron. Astrophys., 365, 174-185 (2001)
	Warm H_{2} in the Galactic Center region.
o	Table 1: <GCM +LL.ll+BB.bb> N=8 added.
Ref:	=2001ApJ...548L..65M
by	MARTIN-PINTADO J. , RIZZO J.R., DE VICENTE P., RODRIGUEZ-FERNANDEZ N.J., FUENTE A.
	Astrophys. J., 548, 65-68 (2001)
	Large-scale grain mantle disruption in the Galactic Center.
o	Table 1: <GCM +LL.ll+BB.bb> N=18 added.
Ref:	=2006A&A...455..971R
by	REQUENA-TORRES M.A. , MARTIN-PINTADO J., RODRIGUEZ-FRANCO A., MARTIN S., RODRIGUEZ-FERNANDEZ N.J., DE VICENTE P.
	Astron. Astrophys., 455, 971-985 (2006)
	Organic molecules in the Galactic center. Hot core chemistry without hot cores.
o	Table 2: <GCM +LL .lll+BB.bbb> N=10.
Ref:	=2008ApJ...672..352R
by	REQUENA-TORRES M.A. , MARTIN-PINTADO J., MARTIN S., MORRIS M.R.
	Astrophys. J., 672, 352-360 (2008)
	The Galactic Center: the largest oxygen-bearing organic molecule repository.
o	Table 2: <GCM +LL.ll+BB.bb> N=1 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCM2003]
[GCM2003]	(Goncalves+Corradi+Mampaso+, 2003)
Write:	<<[GCM2003] NGC 7009 AN>>
N:	4+2+3
Object:	Feature (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Morphological components of NGC 7009: Components are detected in HST WFPC2 images, and studied with IDS on the Issac Newton Telescope. (Nos K1-K4) are Knots, (Nos J1-J2) are Jetlike, (Nos R1-R3) are rims.
in source:	NGC 7009
Ref:	=2003ApJ...597..975G
by	GONCALVES D.R. , CORRADI R.L.M., MAMPASO A., PERINOTTO M.
	Astrophys. J., 597, 975-985 (2003)
	The physical parameters, excitation, and chemistry of the rim, jets, and knots of the planetary nebula NGC 7009.
o	(Erratum) erratum vol. 601, p. 1161 (2004)
o	Fig.1: <[GCM2003] NGC 7009 AN> (Nos K1-K4, J1-J2, R1-R3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCM2018]
[GCM2018]	(Galera-Rosillo+Corradi+Mampaso, 2018)= (GMC) = ([GCM2018a])
Write:	<<[GCM2018] N>> <<[GCM2018] ENN>>
N:	8+14
Object:	Poss. PN (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
Stat:	is completely incorporated in Simbad
Note:	INT WFC photometry and WHT 4.2m ACAM spectroscopy observations of N=8+14 planetary nebulae candidates and sources in the disc of M 33.
in source:	M 33 = NGC 598
Ref:	=2018A&A...612A..35G
by	GALERA-ROSILLO R. , CORRADI R.L.M., MAMPASO A.
	Astron. Astrophys., 612A, 35-35 (2018)
	A deep narrowband survey for planetary nebulae at the outskirts of M 33.
o	Table 4: <[GCM2018] N> (Nos 1-8). Table 7: <[GCM2018] ENN> (Nos E1-E14).
o	Table 1 fields not in SIMBAD.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCM2018a]
[GCM2018a]	(Galera-Rosillo+Corradi+Mampaso, 2018)= (GMC)
*****	Avoid the usage of [GCM2018a], prefer [GCM2018]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCM2018b]
[GCM2018b]	(Galbany+Collett+Mendez-Abreu+, 2018)
Write:	<<[GCM2018b] A>>
N:	19
Object:	Grav. lens + Grav. lensed image of a G + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT MUSE observations of N=1 gravitational lens (A), N=2 gravitationally lensed images of a galaxie (B, C), N=15 galaxies and N=1 merger in the field of 2MASX J04035024-0239275.
Ref:	=2018MNRAS.479..262G
by	GALBANY L. , COLLETT T.E., MENDEZ-ABREU J., SANCHEZ S.F., ANDERSON J.P., KUNCARAYAKTI H.
	Mon. Not. R. Astron. Soc., 479, 262-274 (2018)
	Serendipitous discovery of a strong-lensed galaxy in integral field spectroscopy from MUSE.
o	Fig. 1, Table 1: <[GCM2018b] A> (Nos A-S).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCM90]
[GCM90]	(Graham+Carico+Matthews+, 1990)
Write:	<<[GCM90] Arp 220 A>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Double nucleus of APG 220: N=2 resolved sources at 2.2mu.m, source A = western nucleus, source B = eastern nucleus.
in source:	IC 4553 = APG 220
Ref:	=1990ApJ...354L...5G
by	GRAHAM J.R. , CARICO D.P., MATTHEWS K., NEUGEBAUER G., SOIFER B.T., WILSON T.D.
	Astrophys. J., 354, 5-8 (1990)
	The double nucleus of Arp 220 unveiled.
o	<[GCM90] Arp 220 A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCM98]
[GCM98]	(Garcia+Callanan+Moraru+, 1998) (Not yet in Simbad)
Write:	<<[GCM98] Star A>>
N:	2
Object:	* (SIMBAD class: Star)
Note:	N=2 possible optical counterpart to GRB 970508
Ref:	=1998ApJ...500L.105G
by	GARCIA M.R. , CALLANAN P.J., MORARU D., McCLINTOCK J.E., TOLLESTRUP E., WILLNER S.P., HERGENROTHER C., ROBINSON C.R., KOUVELIOTOU C., VAN PARADIJS J.
	Astrophys. J., 500, 105-110 (1998)
	Power-law decays in the optical counterparts of GRB 970228 and GRB 970508.
o	Table 1: <[GCM98] Star A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCN2010]
[GCN2010]	(Garg+Cook+Nikolaev+, 2010)
Write:	<<[GCN2010] NNNNN-smFF-NN>> <<[GCN2010] NNNNN-smaF-NN>> <<[GCN2010] NNNNN-smaa-NN>> <<[GCN2010] NNNNN_smFF_NN>> (not recognised by Simbad, but found in literature) <<[GCN2010] NNNNN_smaF_NN>> <<[GCN2010] NNNNN_smaa_NN>>
N:	2323
Object:	Poss. delta Scuti * (SIMBAD class: delSctV* = delta Sct Variable)
Note:	CTIO Blanco 4m telescope MOSAIC II observations of N=2323 δ Scuti candidates in the Large Magellanic Clouds.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2010AJ....140..328G
by	GARG A. , COOK K.H., NIKOLAEV S., HUBER M.E., REST A., BECKER A.C., CHALLIS P., CLOCCHIATTI A., MIKNAITIS G., MINNITI D., MORELLI L., OLSEN K., PRIETO J.L., SUNTZEFF N.B., WELCH D.L., WOOD-VASEY W.M.
	Astron. J., 140, 328-338 (2010)
	High-amplitude δ-Scutis in the Large Magellanic Cloud.
o	Table 1: <[GCN2010] NNNNN-smFF-NN>, <[GCN2010] NNNNN-smaF-NN>, <[GCN2010] NNNNN-smaa-NN> N=2323.
=E=	Catalogue in electronic form as <J/AJ/140/328/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCN98]
[GCN98]	(Giovannetti+Caux+Nadeau+, 1998)
====>	Equivalent to: GCNM
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GCNM
GCNM	(Giovannetti+Caux+Nadeau+Monin)= [GCN98]
Write:	<<GCNM NNN>>
N:	165
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	NAME Serpens Cloud
Ref:	=1998A&A...330..990G
by	GIOVANNETTI P. , CAUX E., NADEAU D., MONIN J.-L.
	Astron. Astrophys., 330, 990-998 (1998)
	Deep optical and near infrared imaging photometry of the Serpens cloud core.
o	Table 2: <GCNM NNN> (Nos 1-165).
=E=	Catalogue in electronic form as J/A+A/330/990
Origin	of the Acronym: L (1999AJ....118..558K)
History	of this Acronym: replaces [GCN98]
Details on Acronym: [GCP2006]
[GCP2006]	(Georgakakis+Chavushyan+Plionis+, 2006)
Write:	<<[GCP2006] ANNN>>
N:	32
Object:	AGN (SIMBAD class: Galaxy)
Note:	XMM-Newton Serendipitous Source Catalog to identified normal galaxy candidates.
Ref:	=2006MNRAS.367.1017G
by	GEORGAKAKIS A.E. , CHAVUSHYAN V., PLIONIS M., GEORGANTOPOULOS I., KOULOURIDIS E., LEONIDAKI I., MERCADO A.
	Mon. Not. R. Astron. Soc., 367, 1017-1028 (2006)
	Mining for normal galaxies in the first XMM-Newton Serendipitous Source Catalog.
o	Table 1: <[GCP2006] ANNN> N=32 among (Nos A001-A173).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GCPS
GCPS	(Gal Center P-band Survey)
Write:	<<GCPS NNN>> <<GCPS GLLL.lll+B.bbb>>
N:	241
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA image of the Galactic Center region at 330MHz. See also NTF.
in source:	NAME Gal Center
Ref:	=2004AJ....128.1646N
by	NORD M.E. , LAZIO T.J.W., KASSIM N.E., HYMAN S.D., LAROSA T.N., BROGAN C.L., DURIC N.
	Astron. J., 128, 1646-1670 (2004)
	High-resolution, wide-field imaging of the Galactic Center region at 330 MHz.
o	(Erratum) erratum vol. 131, 1886 (2006)
o	Table 2: <GCPS NNN> (Nos 1-241) = <GCPS GLLL.lll+B.bbb> N=241.
=E=	Catalogue in electronic form as J/AJ/128/1646
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCR2001]
[GCR2001]	(Gray+Cohen+Richards+, 2001)
Write:	<<[GCR2001] Spot A>>
N:	4
Object:	OH Maser (SIMBAD class: Maser)
Note:	MERLIN observations of OH maser emission in W 3(OH).
in source:	W 3:W 3(OH) = W 3(OH)
Ref:	=2001MNRAS.324..643G
by	GRAY M.D. , COHEN R.J., RICHARDS A.M.S., YATES J.A., FIELD D.
	Mon. Not. R. Astron. Soc., 324, 643-647 (2001)
	Co-propagation of maser emission at 1720 and 4765 MHz.
o	Table 1: <[GCR2001] Spot A> (Nos A-D)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCR2002]
[GCR2002]	(Girart+Curiel+Rodriguez+, 2002)= (VLA)
Write:	<<[GCR2002] HH NN-NN VLA N>> <<[GCR2002] NGC 2264D VLA NN>> <<[GCR2002] LNNNNA VLA N>> <<[GCR2002] V645 Cyg VLA N>> <<[GCR2002] MWC 1080 VLA N>>
N:	6+12+7+8+6+1+1+3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA continuum observations towards 8 star forming regions.
Ref:	=2002RMxAA..38..169G
by	GIRART J.M. , CURIEL S., RODRIGUEZ L.F., CANTO J.
	Rev. Mex. Astron. Astrofis., 38, 169-186 (2002)
	Radio continuum observations towards optical and molecular outflows.
o	IRS A, B, C = [[MRC90] IRS A, B, C. Table 4: IRAS 06328+0939 is a misprint for IRAS 06382+0939. in ref list WILKING B.A., CLAUSSEN M.J. 198 7ApJ...320L.133W
o	Tables 2, 3, 4: <[GCR2002] HH 94-95 VLA N> (Nos 1-6), <[GCR2002] NGC 2264D VLA NN> (Nos 1-12), <[GCR2002] L778 VLA N> (Nos 1-7), <[GCR2002] V645 Cyg VLA N> (Nos 1-8), <[GCR2002] MWC 1080 VLA N> (Nos 1-6), <[GCR2002] L1489 VLA N> (No. 1), <[GCR2002] HH 68-69 VLA N> (No. 1), <[GCR2002] L1681B VLA N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCR2006]
[GCR2006]	(Gorosabel+Castro-Tirado+Ramirez-Ruiz+, 2006) (Not yet in Simbad)
Write:	<<[GCR2006] A>>
N:	4
Object:	* (SIMBAD class: Star)
Note:	Reference stars in the field of GRB 030329.
Ref:	=2006ApJ...641L..13G
by	GOROSABEL J. , CASTRO-TIRADO A.J., RAMIREZ-RUIZ E., GRANOT J., CAON N., CAIROS L.M., RUBIO-HERRERA E., GUZIY S., DE UGARTE POSTIGO A., JELINEK M.
	Astrophys. J., 641, 13-16 (2006)
	Revealing the jet structure of GRB 030329 with high-resolution multicolor photometry.
o	Fig.1: <[GCR2006] A> (Nos A-D).
=E=	Catalogue in electronic form as J/ApJ/641/L13
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCR2008]
[GCR2008]	(Gonzalez Hernandez+Caballero+Rebolo+, 2008)= (SO)
Write:	<<[GCR2008] NNNNNN>>
N:	24
Object:	* in Cl* (SIMBAD class: Star)
Note:	WHT WYFFOS observations of N=24 stars from the Caballero Thesis (2006), used to investigate the metallicity of the sig Ori Cluster.
in source:	NAME sig Ori Cluster
Ref:	=2008A&A...490.1135G
by	GONZALEZ HERNANDEZ J.I. , CABALLERO J.A., REBOLO R., BEJAR V.J.S., BARRADO Y NAVASCUES D., MARTIN E.L., ZAPATERO OSORIO M.R.
	Astron. Astrophys., 490, 1135-1142 (2008)
	Chemical abundances of late-type pre-main sequence stars in the σ Orionis cluster.
o	Table 2 [SWW2004] 125 is [SWW2004] J053751.521-023525.55 in Simbad.
o	Table 1: <[GCR2008] NNNNNN> N=24 among (Nos 6-440660).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCR2019]
[GCR2019]	(Gregory+Collins+Read+, 2019)
Write:	<<[GCR2019] NNNNNN>>
N:	131
Object:	* (SIMBAD class: Star)
Note:	Magellan Clay telescope Megacam photometry and VLT FLAMES+GIRAFFE spectroscopy of N=131 stars in the Tucana Dwarf Galaxy.
in source:	NAME Tucana Dwarf Galaxy
Ref:	=2019MNRAS.485.2010G
by	GREGORY A.L. , COLLINS M.L.M., READ J.I., IRWIN M.J., IBATA R.A., MARTIN N.F., McCONNACHIE A.W., WEISZ D.R.
	Mon. Not. R. Astron. Soc., 485, 2010-2025 (2019)
	Kinematics of the Tucana Dwarf Galaxy: an unusually dense dwarf in the Local Group.
o	Tables 2-3: <[GCR2019] NNNNNN> N=131 among (Nos 4032-100021).
=E=	Catalogue in electronic form as <J/MNRAS/485/2010/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCR94]
[GCR94]	(Griffiths+Casertano+Ratnatunga+, 1994)
Write:	<<[GCR94] 1-NN>> <<[GCR94] 2-NN>> <<[GCR94] 3-NN>>
N:	10+15+20
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Observed with HST Planetary WFC 2. Plate L8, Fig 1: format '1-NN', N=10. Plate L9, Fig 2: format '2-NN', N=15. Plate L10, Fig 3: format '3-NN', N=20.
Ref:	=1994ApJ...435L..19G
by	GRIFFITHS R.E. , CASERTANO S., RATNATUNGA K.U., NEUSCHAEFER L.W., ELLIS R.S., GILMORE G.F., GLAZEBROOK K., SANTIAGO B., HUCHRA J.P., WINDHORST R.A., PASCARELLE S.M., GREEN R.F., ILLINGWORTH G.D., KOO D.C., TYSON A.J.
	Astrophys. J., 435, 19-22 (1994)
	The morphology of faint galaxies in medium deep survey images using WFPC2.
o	Plate L8, Fig 1: <[GCR94] 1-NN> N=10, Plate L9, Fig 2: <[GCR94] 2-NN> N=15, Plate L10, Fig 3: <[GCR94] 3-NN> N=20
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GCRT
GCRT	(Galactic Center Radio Transient)
Write:	<<GCRT JHHMM+DDMM>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	New radio transients in the Galactic Center.
in source:	NAME Galactic Center
Ref:	=2002AJ....123.1497H
by	HYMAN S.D. , LAZIO T.J.W., KASSIM N.E., BARTLESON A.L.
	Astron. J., 123, 1497-1501 (2002)
	Low-frequency radio transients in the Galactic Center.
o	<GCRT JHHMM+DDMM> N=1.
Ref:	=2005Natur.434...50H
by	HYMAN S.D. , LAZIO T.J.W., KASSIM N.E., RAY P.S., MARKWARDT C.B., YUSEF-ZADEH F.
	Nature, 434, 50-52 (2005)
	A powerful bursting radio source towards the Galactic Centre.
o	2MASS 0036+18 = 2MASSW J0036159+182110, DENIS 1048-3956 = DENIS-P J104814.7-395606, p. 52 : 3EG J1744-301 is 3EG J1744-3011
o	<GCRT JHHMM+DDMM> N=1.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GCRV
GCRV	(General Catalog of stellar Radial Velocities)= (W) = (Wil) = (Wils) = (Wilson)
Write:	<<GCRV NNNNN>>
N:	15106+8377
Object:	* (SIMBAD class: Star)
Stat.	in SIMBAD: Wilson's catalog is completely incorporated (Cat. III/21).
Note:	The General Catalogue of Stellar Radial Velocity is a compilation of the radial velocities for about 15,000 stars. In SIMBAD, the acronym has been extended (numbers≥50000) for referencing stars having radial velocities published later, and compiled by Abt & Biggs in 1972 (VizieR Cat. III/4).
Ref:	=1953GCRV..C......0W
by	WILSON R.E.
	Carnegie Inst. Washington D.C. Publ. 601, 0-None (1953)
	General Catalogue of Stellar Radial Velocities.
o	<GCRV NNNNN> N=15106.
=E=	Catalogue in electronic form as III/21
=E=	Catalogue in electronic form as III/4
Details on Acronym: GCS
GCS	(Gal. Center Source)
Write:	<<GCS NN>> <<GCS A>> <<GCS 3-N>>
N:	10+30+4
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	(Nos A-J): diffuse sources. (Nos 1-30): dicrete sources. (Nos 3-1 to 3-4) and No. 4 are the five members of a peculiar infrared quintuplet source, along the light of sight towards the Gal. Center Radio Arc. The 4 sources GSC 3-1 to 3-4 are sometimes found with a roman numeral, as '3 I' to '3 IV' sources. See also [NWS90].
Ref:	=1983PASJ...35..101K
by	KOBAYASHI Y. , OKUDA H., SATO S., JUGAKU J., DYCK H.M.
	Publ. Astron. Soc. Jap., 35, 101-112 (1983)
	Infrared polarization in the direction to the Galactic Center.
o	Table 1: <GCS A> (Nos A-J), Table 2: <GCS NN> (Nos 1-15)
Ref:	=1990ApJ...351...83N
by	NAGATA T. , WOODWARD C.E., SHURE M., PIPHER J.L., OKUDA H.
	Astrophys. J., 351, 83-88 (1990)
	AFGL 2004: an infrared Quintuplet near the Galactic Center.
o	Table 1: <GCS 3-N> (Nos 3-1 to 3-4). Table 2: <[NWS90] A> (Nos A-I).
Ref:	=2009ApJS..181..110M
by	MUNO M.P. , BAUER F.E., BAGANOFF F.K., BANDYOPADHYAY R.M., BOWER G.C., BRANDT W.N., BROOS P.S., COTERA A., EIKENBERRY S.S., GARMIRE G.P., HYMAN S.D., KASSIM N.E., LANG C.C., LAZIO T.J.W., LAW C., MAUERHAN J.C., MORRIS M.R., NAGATA T., NISHIYAMA S., PARK S., RAMIREZ S.V., STOLOVY S.R., WIJNANDS R., WANG Q.D., WANG Z., YUSEF-ZADEH F.
	Astrophys. J., Suppl. Ser., 181, 110-128 (2009)
	A catalog of X-ray point sources from two megaseconds of Chandra observations of the Galactic center.
o	Table 2, col(1): numbering NNNN not used in SIMBAD.
o	Table 1: <GCS NN> (Nos 16-30) added. Table 2, col(2): <CXOGC JHHMMSS.s+DDMMSS> N=9017.
=E=	Catalogue in electronic form as <J/ApJS/181/110/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GCS
GCS	(Galactic Center Shell)
*****	Avoid the usage of GCS, prefer [S2003c]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GCS2005]
[GCS2005]	(Garcia-Burillo+Combes+Schinnerer+, 2005)
Write:	<<[GCS2005] JHHMMSS.ss+DDMMSS.s>>
N:	4
Object:	AGN (SIMBAD class: AGN = Active Galaxy Nucleus)
Stat:	is completely incorporated in Simbad
Note:	IRAM PdB CO observations of 4 AGNs in galaxy nucleus as part of the NUGA (Nucleus of Galaxies) CO project.
in source:	NGC 4321
in source:	NGC 4826
in source:	NGC 4579
in source:	NGC 6951
Ref:	=2005A&A...441.1011G
by	GARCIA-BURILLO S. , COMBES F., SCHINNERER E., BOONE F., HUNT L.K.
	Astron. Astrophys., 441, 1011-1030 (2005)
	Molecular gas in NUclei of GAlaxies (NUGA). IV. Gravitational torques and AGN feeding.
o	Figs 1-4: <[GCS2005] JHHMMSS.ss+DDMMSS.s> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCS2006]
[GCS2006]	(Grocholski+Cole+Sarajedini+, 2006)
Write:	<<[GCS2006] SL NNN NN>> <<[GCS2006] Reticulum NN>> <<[GCS2006] Hodge NN NN>>
N:	74
Object:	* in Cl* (SIMBAD class: Star)
Note:	VLT FORS2 observations. Search for stars in 9 stellar clusters. For NGC and IC clusters, the designation is: Cl* NGC NNNN GCS NN, and Cl* IC 2146 GCS NN.
in source:	[SL63] 4
in source:	[SL63] 41
in source:	[SL63] 396
in source:	[SL63] 663
in source:	[SL63] 869
in source:	NAME Reticulum Cluster
in source:	[H60b] 3
in source:	[H60b] 4
in source:	[H60b] 11
Ref:	=2006AJ....132.1630G
by	GROCHOLSKI A.J. , COLE A.A., SARAJEDINI A., GEISLER D., SMITH V.V.
	Astron. J., 132, 1630-1644 (2006)
	Ca II triplet spectroscopy of Large Magellanic Cloud red giants. I. Abundances and velocities for a sample of populous clusters.
o	Table 3: <[GCS2006] SL NNN NN>, <[GCS2006] Reticulum NN>, <[GCS2006] Hodge NN NN>, N=74. Table 3: <Cl* NGC NNNN GCS NN> N=146, <Cl* IC 2146 GCS NN> N=18 among (Nos 2-21).
=E=	Catalogue in electronic form as J/AJ/132/1630
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCS2008]
[GCS2008]	(Gruendi+Chu+Seale+, 2008)
Write:	<<[GCS2008] JHHMMSS.ss+DDMMSS.s>>
N:	13
Object:	AB* (SIMBAD class: AGB* = Asymptotic Giant Branch Star)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC and MIPS observations of the LMC. Discovery of N=13 extreme carbon stars.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2008ApJ...688L...9G
by	GRUENDL R.A. , CHU Y.-H., SEALE J.P., MATSUURA M., SPECK A.K., SLOAN G.C., LOONEY L.W.
	Astrophys. J., 688L, 9-12 (2008)
	Discovery of extreme carbon stars in the Large Magellanic Cloud.
o	Table 1: <[GCS2008] JHHMMSS.ss+DDMMSS.s> N=13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCS90]
[GCS90]	(Gosset+Clowes+Surdej+, 1990)
Write:	<<[GCS90] NNN>>
N:	175
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Note:	QSO candidates around NGC 520.
Ref:	=1990MNRAS.245...71G
by	GOSSET E. , CLOWES R.G., SURDEJ J., SWINGS J.P.
	Mon. Not. R. Astron. Soc., 245, 71-81 (1990)
	A search for quasars in a field around NGC 520.
o	Table 3: <[GCS90] NNN> (Nos 1-175)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCS95]
[GCS95]	(Gagne+Caillault+Stauffer, 1995)
Write:	<<[GCS95] NNN>>
N:	389
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations. Fig. 2: maps
in source:	NAME Orion Nebula
Ref:	=1995ApJ...445..280G
by	GAGNE M. , CAILLAULT J.-P., STAUFFER J.R.
	Astrophys. J., 445, 280-313 (1995)
	Deep ROSAT HRI observations of the Orion nebula region.
o	(Erratum) Erratum Vol. 482, p. 569
o	Table 3: cross-id. H24 not identified
o	<[GCS95] NNN> (Nos 1-389)
=E=	Catalogue in electronic form as J/ApJ/445/280
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCS98]
[GCS98]	(Germany+Chan+Sabine, 1998)
Write:	<<[GCS98] JHHMMSS.ss+DDMMSS.s>>
N:	2
Object:	G + * (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=1 host galaxy of SN 1998CH, J132914.41-291728.6, and N=1 nearby *, J132914.53-291652.6
Ref:	=1998IAUC.6917R...1G
by	GERMANY L. , (The Mount Stromlo Abell Cluster Supernova Search Team), CHAN S., SABINE S.
	IAU Circ., 6917, 1-None (1998)
	Supernova 1998ch in anonymous galaxy.
o	<[GCS98] J132913.41-291725.0>, <[GCS98] J132914.53-291652.6>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GCSS
GCSS	(General Catalog of S Stars)
**	catalog: use S1*
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GCT2005]
[GCT2005]	(Giordano+Cortese+Trinchieri+, 2005)
Write:	<<[GCT2005] NN>>
N:	54
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of NGC 4261.
in source:	NGC 4261
Ref:	=2005ApJ...634..272G
by	GIORDANO L. , CORTESE L., TRINCHIERI G., WOLTER A., COLPI M., GAVAZZI G., MAYER L.
	Astrophys. J., 634, 272-280 (2005)
	The trail of discrete X-ray sources in the early-type galaxy NGC 4261: anisotropy in the globular cluster distribution?
o	Table 2: <[GCT2005] NN> (Nos 1-54).
=E=	Catalogue in electronic form as J/ApJ/634/272
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GCT94]
[GCT94]	(Gomez+Curiel+Torrelles+, 1994)= (VLA)
Write:	<<[GCT94] VLA N>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
in source:	NGC 2264G
Ref:	=1994ApJ...436..749G
by	GOMEZ J.F. , CURIEL S., TORRELLES J.M., RODRIGUEZ L.F., ANGLADA G., GIRART J.M.
	Astrophys. J., 436, 749-753 (1994)
	The molecular core and the powering source of the bipolar molecular outflow in NGC 2264G.
o	'NGC 2264G = [MLS88] G' . p.750: calibrators 0725+144 et 0550+032 not in SIMBAD
o	<[GCT94] VLA N> N=2
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GCTP
GCTP	(General Catalog of Trigon. stellar Parallaxes)
*****	Avoid the usage of GCTP, prefer PLX
Details on Acronym: GCVS
GCVS	(General Catalog of Variable *)
*****	Avoid the usage of GCVS, prefer EV*
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GCVS
GCVS	(General Catalog of Variable *)
====>	Equivalent to: V*
Details on Acronym: [GCW98]
[GCW98]	(Gorosabel+Castro-Tirado+Wolf+, 1998)
Write:	<<[GCW98] GRB 970111 N>> <<[GCW98] SAX J1528.8+1944 NN>> <<[GCW98] SAX J1528.8+1937 NN>>
N:	9+12+17
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 5: N=9 objects in the error box of GRB 970111, map in Fig.2. Table 6: N=12 objects in the error box of SAX J1528.8+1944, map in Fig.4a. No. 11 could be the optical counterpart of SAX object. Table 6: N=17 objects in the error box of SAX J1528.8+1937, map in Fig.4b. No. 4 could be the optical counterpart of SAX object.
Ref:	=1998A&A...339..719G
by	GOROSABEL J. , CASTRO-TIRADO A.J., WOLF C., HEIDT J., SEITZ T., THOMMES E., BARTOLINI C., GUARNIERI A., MASETTI N., PICCIONI A., LARSEN S., COSTA E., FEROCI M., FRONTERA F., PALAZZI E., LUND N.
	Astron. Astrophys., 339, 719-728 (1998)
	An optical study of the GRB 970111 field beginning 19 hours after the γ-ray burst.
o	Table 5: <[GCW98] GRB 970111 N> (Nos 1-9). Table 6: <[GCW98] SAX J1528.8+1944 NN> (Nos 1-12). Table 7: <[GCW98] SAX J1528.8+1937 NN> (Nos 1-17).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GD
GD	(Giclas, Dwarf)
Write:	<<GD NNNNA>>
N:	1712
Object:	Susp. WD + Blue * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	1980LowOB...8..157G: Recapitulation of the complete catalogue in order of right ascension.
Ref:	=1965LowOB...6..155G
by	GICLAS H.L. , BURNHAM R., THOMAS N.G.
	Lowell Obs. Bull., 6, 155-164 (1965)
	List of white dwarf suspects.
o	<GD NNN> (Nos 1-272)
Ref:	=1967LowOB...7...49G
by	GICLAS H.L. , BURNHAM R., THOMAS N.G.
	Lowell Obs. Bull., 7, 49-54 (1967)
	A list of white dwarf suspects. II.
o	<GD NNN> (Nos 273-407)
Ref:	=1970LowOB...7..183G
by	GICLAS H.L. , BURNHAM R., THOMAS N.G.
	Lowell Obs. Bull., 7, 183-189 (1970)
	A list of white dwarf suspects. III.
o	<GD NNN> (Nos 408-562)
Ref:	=1972LowOB...7..217G
by	GICLAS H.L. , BURNHAM R., THOMAS N.G.
	Lowell Obs. Bull., 7, 217-254 (1972)
	Proper motion survey at the South Galactic Pole. Lists of white dwarf suspects. List of very red stars.
o	Plates 266-269
o	<GR* NN> (Nos 1-47). <GD NNN> (Nos 563-952)
Ref:	=1975LowOB...8....9G
by	GICLAS H.L. , BURNHAM R., THOMAS N.G.
	Lowell Obs. Bull., 8, 9-49 (1975)
	Lowell proper motions. XVII.
o	Plates 272-273
o	<GR* NNN> (Nos 120-288). <GD NNNN> (Nos 953-1338).
Ref:	=1978LowOB...8...51G
by	GICLAS H.L. , BURNHAM R., THOMAS N.G.
	Lowell Obs. Bull., 8, 51-88 (1978)
	Lowell proper motions. XVIII.
o	Plates 274-275
o	<GR* NNN> (Nos 289-504). <GD NNNN> (Nos 1339-1712)
=E=	Catalogue in electronic form as <I/316/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GD2000]
[GD2000]	(Gaztanaga+Dalton, 2000) (Not yet in Simbad)
Write:	<<[GD2000] N>>
N:	9
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	N=9 Zwicky galaxies.
Ref:	=2000MNRAS.312..417G
by	GAZTANAGA E. , DALTON G.B.
	Mon. Not. R. Astron. Soc., 312, 417-428 (2000)
	On the CCD calibration of Zwicky galaxy magnitudes and the properties of nearby field galaxies.
o	Table 3, Figs 11 et 12: <[GD2000] N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GD2012]
[GD2012]	(Grosbol+Dottori, 2012)
Write:	<<[GD2012] NGCNNNN NNNN>>
N:	25520 (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	VLT HAWK-I NIR observations of N=10 nearby, grand-design, spiral galaxies.
in source:	NGC 157
in source:	NGC 1232
in source:	NGC 1300
in source:	NGC 1365
in source:	NGC 1566
in source:	NGC 2997
in source:	NGC 4030
in source:	NGC 4321
in source:	NGC 5247
in source:	NGC 7424
Ref:	=2012A&A...542A..39G
by	GROSBOL P. , DOTTORI H.
	Astron. Astrophys., 542A, 39-39 (2012)
	Star formation in grand-design, spiral galaxies. Young, massive clusters in the near-infrared.
o	<[GD2012] NGCNNNN NNNN> N=25520
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GD2021]
[GD2021]	(Gusev+Dodin, 2021)
Write:	<<[GD2021] NGC NNNN NN>>
N:	23+9
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	2.5-m telescope of the Caucasus Mountain Observatory TDS (Transient Double-beam Spectrograph) observations of N=23+9 HII regions in NGC 3963 and NGC 7292 respectively.
in source:	NGC 3963
in source:	NGC 7292
Ref:	=2021MNRAS.505.2009G
by	GUSEV A.S. , DODIN A.V.
	Mon. Not. R. Astron. Soc., 505, 2009-2019 (2021)
	Peculiarities of the chemical abundance distribution in galaxies NGC 3963 and NGC 7292.
o	Fig. 1, Tables 3-5: <[GD2021] NGC 3963 NN> (Nos 1-23), <[GD2021] NGC 7292 N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GD77]
[GD77]	(Genzel+Downes, 1977)
Write:	<<[GD77] A>>
N:	2
Object:	H2O Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
in source:	NAME Orion Nebula
Ref:	=1977A&A....61..117G
by	GENZEL R. , DOWNES D.
	Astron. Astrophys., 61, 117-126 (1977)
	H2O in Orion: outflow of matter in the last stages of star formation.
o	<[GD77] A> (Nos A-B)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GD98]
[GD98]	(Galaz+De Lapparent, 1998)
Write:	<<[GD98] 7-NN>> <<[GD98] 8-N>>
N:	42
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Table 7: Brightest galaxies, format '7-NN' (Nos 7-1 to 7-38), with No. 2 = No. 3, No. 10 = No. 11 = No. 12 Table 8: Peculiar objects, format '8-N' (Nos 8-1 to 8-9)
Ref:	=1998A&A...332..459G
by	GALAZ G. , DE LAPPARENT V.
	Astron. Astrophys., 332, 459-478 (1998)
	The ESO-Sculptor Survey: spectral classification of galaxies with z ≲ 0.5.
o	Table 7: <[GD98] 7-NN> (Nos 7-1 to 7-38). Table 8: <[GD98] 8-N> (Nos 8-1 to 8-9)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDB2006]
[GDB2006]	(Gouliermis+Dolphin Brandner+, 2006)
Write:	<<[GDB2006] NNNNN>>
N:	99079
Object:	* (SIMBAD class: Star)
Note:	Archival HST ACS photometric observations of the region of NGC 346.
in source:	Magellanic Clouds:SMC:NGC 346 = NGC 346
Ref:	=2006ApJS..166..549G
by	GOULIERMIS D.A. , DOLPHIN A.E., BRANDNER W., HENNING T.
	Astrophys. J., Suppl. Ser., 166, 549-556 (2006)
	The star-forming region NGC 346 in the Small Magellanic Cloud with Hubble space telescope ACS observations. I. Photometry.
o	Table 2: <[GDB2006] NNNNN> (Nos 1-99079).
=E=	Catalogue in electronic form as J/ApJS/166/549
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDB2008]
[GDB2008]	(Grove+Da Costa+Benoist, 2008)
Write:	<<[GDB2008] NNN>>
N:	747
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	La Silla Danish 1.54m telescope spectroscopy of N=747 galaxies in N=23 [OSD99] cluster fields.
Ref:	=2008A&A...490..945G
by	GROVE L.F. , DA COSTA L., BENOIST C.
	Astron. Astrophys., 490, 945-963 (2008)
	Multi-object spectroscopy of low-redshift EIS clusters. IV. Reliability of matched-filter results at z ~ 0.3-0.4.
o	Table 1: <[OSD99] EIS JHHMM+DDMMA> N=4 added. Table 3: <[GDB2008] NNN> (Nos 1-747).
=E=	Catalogue in electronic form as J/A+A/490/945
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDB2015]
[GDB2015]	(Gonzalez+Decker+Brodwin+, 2015)
Write:	<<[GDB2015] JHHMMSS.ss+DDMMSS.s>>
N:	15
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Gemini-North GMOS and Keck DEIMOS and MOSFIRE spectroscopy of N=15 galaxies in the field of the galaxy cluster MOO J1142+1527. See also [GGS2012] and [GGB2019].
in source:	MOO J1142+1527
Ref:	=2015ApJ...812L..40G
by	GONZALEZ A.H. , DECKER B., BRODWIN M., EISENHARDT P.R.M., MARRONE D.P., STANFORD S.A., STERN D., WYLEZALEK D., ALDERING G., ABDULLA Z., BOONE K., CARLSTROM J., FAGRELIUS P., GETTINGS D.P., GREER C.H., HAYDEN B., LEITCH E.M., LIN Y.-T., MANTZ A.B., MUCHOVEJ S., PERLMUTTER S., ZEIMANN G.R.
	Astrophys. J., 812L, 40 (2015)
	The massive and distant clusters of WISE survey: MOO J1142+1527, a 10^{15} M_☉ galaxy cluster at z = 1.19.
o	<MOO J1142+1527> N=1. Table 1: <[GDB2015] JHHMMSS.ss+DDMMSS.s> N=15.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GDC
GDC	(Gum Dark Cloud)
Write:	<<GDC N>>
N:	7
Object:	Dark Cloud (SIMBAD class: DarkNeb = Dark Cloud (nebula))
Stat:	is completely incorporated in Simbad
Ref:	=1983A&A...117..183R
by	REIPURTH B.
	Astron. Astrophys., 117, 183-198 (1983)
	Star formation in Bok globules and low-mass clouds.
o	<CG NNA> (Nos 37, 38) and 31D, E. <GDC N> (Nos 1-7)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GDC2008]
[GDC2008]	(Greco+Dall'Ora+Clementini+, 2008)
Write:	<<[GDC2008] VN>>
N:	2
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Stat:	is completely incorporated in Simbad
Note:	WHT and WIRO 2.3m telescope observations. Detection of N=2 variable stars in the CVn II dSph galaxy.
in source:	NAME CVn II dSph
Ref:	=2008ApJ...675L..73G
by	GRECO C. , DALL'ORA M., CLEMENTINI G., RIPEPI V., DI FABRIZIO L., KINEMUCHI K., MARCONI M., MUSELLA I., SMITH H.A., RODGERS C.T., KUEHN C., BEERS T.C., CATELAN M., PRITZL B.J.
	Astrophys. J., 675L, 73-76 (2008)
	On the newly discovered Canes Venatici II dSph galaxy.
o	Table 1: <[GDC2008] VN> (Nos V1-V2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDC91]
[GDC91]	(Garcia-Barreto+Downes+Combes, 1991)
Write:	<<[GDC91] N>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=3 background radio-sources in the field of NGC 1022.
Ref:	=1991A&A...252...19G
by	GARCIA-BARRETO J.A. , DOWNES D., COMBES F., CARRASCO L., GERIN M., CRUZ-GONZALEZ I.
	Astron. Astrophys., 252, 19-26 (1991)
	Circumnuclear star formation in the barred galaxy NGC 1022.
o	Table 2: <[GDC91] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDD2007]
[GDD2007]	(Gimeno+Dottori+Diaz+, 2007) (Not yet in Simbad)
Write:	<<[GDD2007] ESO 381-23 NN>> <<[GDD2007] MCG -3-35-14 Condensation>>
N:	3+1
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Search for double nucleus in ESO 381-23 and MCG -3-35-14. N2 and N3 in ESO 381-23 are HII regions.
in source:	ESO 381-23
in source:	MCG-03-35-014
Ref:	=2007AJ....133.2327G
by	GIMENO G.N. , DOTTORI H.A., DIAZ R.J., RODRIGUES I., CARRANZA G.J.
	Astron. J., 133, 2327-2333 (2007)
	Photometry and kinematics of two minor merger candidate galaxies.
o	Table 1, Fig.3: <[GDD2007] ESO 381-23 AN> (Nos N1-N3). Table 3, Fig.7: <[GDD2007] MCG -3-35-14 Condensation> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDD2014]
[GDD2014]	(Graham+Djorgovski+Drake+, 2014)
Write:	<<[GDD2014] QC JHHMM+DDMM>> <<[GDD2014] QCHHMM+DDMM>> (not recognised by Simbad, but found in literature)
N:	20
Object:	QSO + Poss. QSO (SIMBAD class: QSO = Quasar)
Note:	Keck DEIMOS and Palomar 200-in DBSP spectroscopy of N=20 quasar candidates (19 were confirmed).
Ref:	=2014MNRAS.439..703G
by	GRAHAM M.J. , DJORGOVSKI S.G., DRAKE A.J., MAHABAL A.A., CHANG M., STERN D., DONALEK C., GLIKMAN E.
	Mon. Not. R. Astron. Soc., 439, 703-718 (2014)
	A novel variability-based method for quasar selection: evidence for a rest-frame ~ 54d characteristic time-scale.
o	Table 6: <[GDD2014] QC JHHMM+DDMM> N=20.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GDDS
GDDS	(Gemini Deep Deep Survey)
Write:	<<GDDS SAHH-NNNN>>
N:	305
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Gemini Deep Deep Survey (GDDS) is an ultradeep redshift survey targeting galaxies between z=1 to z=2. GDDS SA fields have a format in 'HH' RA hours.
Ref:	=2004AJ....127.2455A
by	ABRAHAM R.G. , GLAZEBROOK K., McCARTHY P.J., CRAMPTON D., MUROWINSKI R., JORGENSEN I., ROTH K., HOOK I.M., SAVAGLIO S., CHEN H.-W., MARZKE R.O., CARLBERG R.G.
	Astron. J., 127, 2455-2483 (2004)
	The Gemini Deep Deep Survey. I. Introduction to the survey, catalogs, and composite spectra.
o	Tables 4, 5: <GDDS SAHH-NNNN> N=305.
=E=	Catalogue in electronic form as J/AJ/127/2455
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GDE2009]
[GDE2009]	(Gregg+Drinkwater+Evstigneeva+, 2009)= (UCD)
Write:	<<[GDE2009] UCD NN>>
N:	60
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	AAT 2dF observations of Ultra Compact Dwarf galaxies (UCD in the format) in the Fornax Cluster. See also FCOS, [DJG2000].
in source:	NAME Fornax Cluster
Ref:	=2009AJ....137..498G
by	GREGG M.D. , DRINKWATER M.J., EVSTIGNEEVA E., JUREK R., KARICK A.M., PHILLIPPS S., BRIDGES T., JONES J.B., BEKKI K., COUCH W.J.
	Astron. J., 137, 498-506 (2009)
	A large population of ultra-compact dwarfs and bright intracluster globulars in the Fornax cluster.
o	Table 2: <[GDE2009] UCD NN> (Nos 1-60).
=E=	Catalogue in electronic form as <J/AJ/137/498/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDF98]
[GDF98]	(Giallongo+D'odorico+Fontana+, 1998)
Write:	<<[GDF98] NNN>>
N:	186
Object:	G (SIMBAD class: Galaxy)
Note:	Galaxies in the field of QSO BR 1202-0725
Ref:	=1998AJ....115.2169G
by	GIALLONGO E. , D'ODORICO S., FONTANA A., CRISTIANI S., EGAMI E., HU E., McMAHON R.G.
	Astron. J., 115, 2169-2183 (1998)
	The photometric redshift distribution and evolutionary properties of galaxies up to z ~ 4.5 in the field of the quasar BR 1202-0725.
o	Table 1: <[GDF98] NNN> N=186 among (Nos 4-852).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDF99]
[GDF99]	(Goldman+Delfosse+Forveille+, 1999)
Write:	<<[GDF99] LHS 102B>>
N:	1
Object:	L dwarf (SIMBAD class: BrownD* = Brown Dwarf)
Stat:	is completely incorporated in Simbad
Note:	EROS 2 and DENIS observations of an L dwarf companion of LHS 102.
Ref:	=1999A&A...351L...5G
by	GOLDMAN B. , DELFOSSE X., FORVEILLE T., AFONSO C., ALARD C., ALBERT J.N., ANDERSEN J., ANSARI R., AUBOURG E., BAREYRE P., BAUER F., BEAULIEU J.P., BORSENBERGER J., BOUQUET A., CHAR S., CHARLOT X., COUCHOT F., COUTURES C., DERUE F., FERLET R., FOUQUE P., GLICENSTEIN J.F., GOULD A., GRAFF D., GROS M., HAISSINSKI J., HAMILTON J.C., HARDIN D., DE KAT J., KIM A., LASSERRE T., LESQUOY E., LOUP C., MAGNEVILLE C., MANSOUX B., MARQUETTE J.B., MARTIN E.L., MAURICE E., MILSZTAJN A., MONIEZ M., PALANQUE-DELABROUILLE N., PERDEREAU O., PREVOT L., REGNAULT N., RICH J., SPIRO M., VIDAL-MADJAR A., VIGROUX L., ZYLBERAJCH S., (The EROS Collaboration)
	Astron. Astrophys., 351, 5-9 (1999)
	EROS 2 proper motion survey: a field brown dwarf, and an L dwarf companion to LHS 102.
o	<EROS-MP JHHMM+DDMM> N=1. <[GDF99] LHS 102B> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDG2000]
[GDG2000]	(Garrett+De Bruyn+Giroletti+, 2000)
Write:	<<[GDG2000] MMSS+MMSS>>
N:	8
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	WSRT 1.4GHz of HDF region. In the format 'MMSS.s-MMSS', relative to 12h and +62deg, (2000 coordinates). See also [RKF98].
in source:	NAME HDFN
Ref:	=2000A&A...361L..41G
by	GARRETT M.A. , DE BRUYN A.G., GIROLETTI M., BAAN W.A., SCHILIZZI R.T.
	Astron. Astrophys., 361, 41-44 (2000)
	WSRT observations of the Hubble Deep Field region.
o	Table 1: <[GDG2000] MMSS+MMSS> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDG2006]
[GDG2006]	(Grosbol+Dottori+Gredel, 2006) (Not yet in Simbad)
Write:	<<[GDG2006] A>>
N:	8
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
Note:	ISAAC on the VLT observations of NGC 2997.
in source:	NGC 2997
Ref:	=2006A&A...453L..25G
by	GROSBOL P. , DOTTORI H., GREDEL R.
	Astron. Astrophys., 453, 25-28 (2006)
	Star-forming knots and density wave in NGC 2997.
o	FIgs 1, 2, Table 1: <[GDG2006] A> (Nos A-H).
Details on Acronym: [GDH2010]
[GDH2010]	(Garcia-Benito+Diaz+Hagele+, 2010) (Not yet in Simbad)
Write:	<<[GDH2010] A>>
N:	4
Object:	Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Calar Alto 3.5m telescope PMAS observations of N=4 knots in NGC 6946.
in source:	NGC 6946
Ref:	=2010MNRAS.408.2234G
by	GARCIA-BENITO R. , DIAZ A., HAGELE G.F., PEREZ-MONTERO E., LOPEZ J., VILCHEZ J.M., PEREZ E., TERLEVICH E., TERLEVICH R., ROSA-GONZALEZ D.
	Mon. Not. R. Astron. Soc., 408, 2234-2255 (2010)
	Integral field spectroscopy of HII region complexes: the outer disc of NGC6946.
o	Fig. 3: <[GDH2010] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDJ2017]
[GDJ2017]	(George+Dwarakanath+Johnston-Hollitt+, 2017)
Write:	<<[GDJ2017] ANNNNa A>> <<[GDJ2017] ANNNN R(W)>> <<[GDJ2017] PLCK G287.0+32.9 H>> <<[GDJ2017] PLCK G287.0+32.9 R(WW)>> <<[GDJ2017] RXC J1314.5-2515 H>> <<[GDJ2017] RXC J1314.5-2515 R(W)>>
N:	21
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Murchison Widefield Array (MWA) observations of radio Haloes H and Relics R in N=9 merging galaxy clusters, as part of the GaLactic and Extragalactic All-sky MWA (GLEAM) Survey.
Ref:	=2017MNRAS.467..936G
by	GEORGE L.T. , DWARAKANATH K.S., JOHNSTON-HOLLITT M., INTEMA H.T., HURLEY-WALKER N., BELL M.E., CALLINGHAM J.R., FOR B.-Q., GAENSLER B., HANCOCK P.J., HINDSON L., KAPINSKA A.D., LENC E., McKINLEY B., MORGAN J., OFFRINGA A., PROCOPIO P., STAVELEY-SMITH L., WAYTH R.B., WU C., ZHENG Q.
	Mon. Not. R. Astron. Soc., 467, 936-949 (2017)
	A study of halo and relic radio emission in merging clusters using the Murchison Widefield Array.
o	Tables 3-4: <[GDJ2017] A13 A> (Nos H and R), <[GDJ2017] A548b A (Nos A-B,H), <[GDJ2017] A2063 A> (Nos H and R), <[GDJ2017] A2163 A> (Nos H and R), <[GDJ2017] A2254 H> N=1, <[GDJ2017] A2345 A(W)> (Nos R(E), R(W) and H), <[GDJ2017] A2744 A> (Nos H and R), <[GDJ2017] PLCK G287.0+32.9 H>, <[GDJ2017] PLCK G287.0+32.9 A(WW)> (Nos R(SE), R(NW) and H), <[GDJ2017] RXC J1314.5-2515 A(W)> (Nos R(E), R(W) and H).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GDK
GDK	(Gordon+Duric+Kirshner+)
*****	Avoid the usage of GDK, prefer [GDK99]
Origin	of the Acronym: L (2001A&A...373..438H)
Details on Acronym: [GDK2005]
[GDK2005]	(Geller+Dell'Antonio+Kurtz+, 2005)
Write:	<<[GDK2005] JHHMMSS+DDMMSS>>
N:	3
Object:	Cl of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	3 ClG part of DLSCL J0920.1+3029. See also [WDH2006]
in source:	ACO 781 = DLSCL J0920.1+3029
Ref:	=2005ApJ...635L.125G
by	GELLER M.J. , DELL'ANTONIO I.P., KURTZ M.J., RAMELLA M., FABRICANT D.G., CALDWELL N., TYSON J.A., WITTMAN D.
	Astrophys. J., 635, 125-128 (2005)
	SHELS: the Hectospec Lensing Survey.
o	<DLSCL JHHMM.m+DDMM> N=1. <[GDK2005] JHHMMSS+DDMMSS> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDK90]
[GDK90]	(Grondin+Demers+Kunkel, 1990)
Write:	<<[GDK90] NNN>>
N:	173
Object:	* in Assoc. (SIMBAD class: Star)
in source:	Magellanic Clouds:Magellanic Bridge = Magellanic Bridge
in source:	IDK 2
Ref:	=1990AJ....100..663G
by	GRONDIN L. , DEMERS S., KUNKEL W.E., IRWIN M.J.
	Astron. J., 100, 663-673 (1990)
	Young stars between the Magellanic Clouds. I. An association at 2h27m, -73°.59'.
o	<[GDK90] NNN> N=173 among (Nos 5-964).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDK92]
[GDK92]	(Grondin+Demers+Kunkel, 1992)
Write:	<<[GDK92] 1-NNN>> <<[GDK92] 3-NNN>> <<[GDK92] 5-NNNN>> <<[GDK92] C-NNN>>
Object:	* in Assoc. (SIMBAD class: Star)
Note:	Table 2: in IDK 1, format '1-NNN', N=118 among 142. Table 3: in IDK 3, format '3-NNN', N=106 among 127. Table 4: in IDK 5, format '5-NNNN', N=118 among 2046. Table 5: Comparison field *, format 'C-NNN', N=118.
in source:	Magellanic Clouds:Magellanic Bridge = Magellanic Bridge
in source:	IDK 1
in source:	IDK 3
in source:	IDK 5
Ref:	=1992AJ....103.1234G
by	GRONDIN L. , DEMERS S., KUNKEL W.E.
	Astron. J., 103, 1234-1251 (1992)
	Young stars between the Magellanic clouds. III. Overall properties of associations : a shallow mass function.
o	Assoc. 1, 3, 5 are respectively IDK 1, 3, 5
o	Table 2, field 1: <[GDK92] 1-NNN> N=118 among (Nos 2-142), Table 3, field 3: <[GDK92] 3-NNN> N=106 among (Nos 1-127), Table 4, field 5: <[GDK92] 5-NNNN> N=118 among (Nos 1-2046), Table 5, comparison: <[GDK92] C-NNN> (Nos 1-118).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDK99]
[GDK99]	(Gordon+Duric+Kirshner+, 1999)= (GDK) = (GDKG)
Write:	<<[GDK99] NNN>>
N:	186
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
in source:	M 33 = NGC 598
Ref:	=1999ApJS..120..247G
by	GORDON S.M. , DURIC N., KIRSHNER R.P., GOSS W.M., VIALLEFOND F.
	Astrophys. J., Suppl. Ser., 120, 247-264 (1999)
	A new sample of radio-selected and optically confirmed supernova remnants in M33.
o	T.2: SNR- = M33SNR, B- = BCLMP, V- = VGHC 2-, G93 = [GBM93]
o	Table 1: <[GDK99] NNN> (Nos 1-186).
=E=	Catalogue in electronic form as J/ApJS/120/247
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GDKG
GDKG	(Gordon+Duric+Kirshner+Goss+)
*****	Avoid the usage of GDKG, prefer [GDK99]
Origin	of the Acronym: L (2001ApJ...559..864J)
Details on Acronym: [GDM2001]
[GDM2001]	(Gaensler+Dickey+McClure-Griffiths+, 2001)
Write:	<<[GDM2001] NN>> <<[GDM2001] Void N>> <<[GDM2001] GLLL.l+B.b>>
N:	21+2+1
Object:	(Rad) + Void + HII (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	SGPS test field: (Nos 1-21), compact sources showing a linear polarization. N=2 large voids in polarization. N=1 HII region, 30' to the lower left of RCW 94, 'G326.7+0.5'.
in source:	NAME SGP
Ref:	=2001ApJ...549..959G
by	GAENSLER B.M. , DICKEY J.M., McCLURE-GRIFFITHS N.M., GREEN A.J., WIERINGA M.H., HAYNES R.F.
	Astrophys. J., 549, 959-978 (2001)
	Radio polarization from the inner galaxy at arcminute resolution.
o	MRC B1438-481 = PMN J1441-4818 ?
o	Table 1: <[GDM2001] NN> (Nos 1-21). Fig.4: <[GDM2001] Void N> (Nos 1-2). Fig.10: <[GDM2001] G326.7+0.5> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDM2005]
[GDM2005]	(Guieu+Dougados+Monin+, 2005)= (CFHT)
Write:	<<[GDM2005] CFHT-VLMS-Tau 1>>
N:	1
Object:	BD* (SIMBAD class: BrownD* = Brown Dwarf)
Stat:	is completely incorporated in Simbad
Note:	CFHT12K imaging of the Taurus star forming region. Use of 2MASS archival data. WHT ISIS spectroscopic follow up. N=1 Very Low Mass Star (VLMS in the format) is found.
in source:	NAME Taurus Region
Ref:	=2005MmSAI..76..253G
by	GUIEU S. , DOUGADOS C., MONIN J.-L., MAGNIER E., MARTIN E.
	Mem. Soc. Astron. Ital., 76, 253-258 (2005)
	Exploring the substellar IMF in the Taurus cloud. New brown dwarfs in the Taurus star forming region.
o	in ref list MARTIN 2001ApJ...561L.195M instead of ApJ.561.195
o	Table 2: <[MDM2001] CFHT-BD-Tau N> (Nos 5-8) added. Table 2: <[GDM2005] CFHT-VLMS-Tau N> (No. 1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDM2010]
[GDM2010]	(Guarcello+Damiani+Micela+, 2010)
Write:	<<[GDM2010] 6611 NNNNN>>
N:	81
Object:	Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Note:	N=81 blue stars with NIR excesses in NGC 6611. Use of Chandra ACIS, UKIDSS, EIS and Spitzer IRAC data. See also Cl* NGC 6611 GPM, Cl* NGC 6611 GMD, [GMP2010].
in source:	NGC 6611 = Eagle Nebula = M 16
Ref:	=2010A&A...521A..18G
by	GUARCELLO M.G. , DAMIANI F., MICELA G., PERES G., PRISINZANO L., SCIORTINO S.
	Astron. Astrophys., 521A, 18-18 (2010)
	Pre-main sequence stars with disks in the Eagle Nebula observed in scattered light.
o	Table: <[GDM2010] 6611 NNNNN> N=81 among (Nos 351-28826).
=E=	Catalogue in electronic form as J/A+A/521/A18
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDN2015]
[GDN2015]	(Gonzalez-Fernandez+Dorda+Negueruela+, 2015)
Write:	<<[GDN2015] SMCNNN>> <<[GDN2015] LMCNNN>>
N:	398+237
Object:	Poss. Red Supergiant (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	AAT 3.9m telescope 2dF/AAOmega spectroscopic observations of N=398+237 red supergiant star candidates in the Magellanic Clouds.
in source:	NAME Magellanic Clouds
in source:	NAME LMC
in source:	NAME SMC
Ref:	=2015A&A...578A...3G
by	GONZALEZ-FERNANDEZ C. , DORDA R., NEGUERUELA I., MARCO A.
	Astron. Astrophys., 578A, 3-3 (2015)
	A new survey of cool supergiants in the Magellanic Clouds.
o	Table A1: <[GDN2015] SMCNNN> N=398 among (Nos 1 to 407), <[GDN2015] LMCNNN> N=237 among (Nos 1 to 264).
=E=	Catalogue in electronic form as J/A+A/578/A3
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDO2000]
[GDO2000]	(Gal+De Carvalho+Odewahn+, 2000)
Write:	<<[GDO2000] FFF NN>>
N:	47+38
Object:	Poss. Cl of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	DPOSS Second Survey. Search for candidate ClG in 2 fields Nos '447' and '475'. Maps in Figs 4 and 5. See also [PAL2001], NSC.
Ref:	=2000AJ....119...12G
by	GAL R.R. , DE CARVALHO R.R., ODEWAHN S.C., DJORGOVSKI S.G., MARGONINER V.E.
	Astron. J., 119, 12-20 (2000)
	The northern sky optical cluster survey. I. Detection of galaxy clusters in DPOSS.
o	Table 1: <[GDO2000] 447 NN> (Nos 1-47). Table 2: <[GDO2000] 475 NN> (Nos 1-38).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDO2011]
[GDO2011]	(Gobat+Daddi+Finoguenov+, 2011)
Write:	<<[GDO2011] NNNN>>
N:	16
Object:	G (SIMBAD class: Galaxy)
Note:	Subaru MOIRCS and VLT ISAAC NIR observations of N=16 red galaxies in the core of ClG J1449+0856.
in source:	ClG J1449+0856
Ref:	=2011A&A...526A.133G
by	GOBAT R. , DADDI E., ONODERA M., FINOGUENOV A., RENZINI A., ARIMOTO N., BOUWENS R., BRUSA M., CHARY R.-R., CIMATTI A., DICKINSON M., KONG X., MIGNOLI M.
	Astron. Astrophys., 526A, 133-133 (2011)
	A mature cluster with X-ray emission at z = 2.07.
o	<ClG J1449+0856> N=1. Table 2: <[GDO2011] NNNN> N=16 among (Nos 4489-5262).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GDP
GDP	(Gregorini+De Ruiter+Parma+)= [GDP94]
Write:	<<GDP ACO NNNN Na>>
N:	252
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 4: Radio-sources in the 93 ACO clusters fields.
Ref:	=1994A&AS..106....1G
by	GREGORINI L. , DE RUITER H.R., PARMA P., SADLER E.M., VETTOLANI G., EKERS R.D.
	Astron. Astrophys., Suppl. Ser., 106, 1-19 (1994)
	Dumbbell galaxies and multiple nuclei in rich clusters: radio data.
o	Table 5 not in SIMBAD
o	Table 4: <GDP ACO NNNN Na> N=252.
=E=	Catalogue in electronic form as J/A+AS/106/1
Origin	of the Acronym: L (1999AJ....118.1131W)
History	of this Acronym: replaces [GDP94]
Details on Acronym: [GDP2000]
[GDP2000]	(Guainazzi+Dennefeld+Piro+, 2000)
Write:	<<[GDP2000] N>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC field of IRAS 12393+3520: N=2 serendipitous sources.
Ref:	=2000A&A...355..113G
by	GUAINAZZI M. , DENNEFELD M., PIRO L., BOLLER T., RAFANELLI P., YAMAUCHI M.
	Astron. Astrophys., 355, 113-120 (2000)
	A direct view of the AGN powering IRAS 12393+3520.
o	Table 1, Fig.2: <[GDP2000] N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDP94]
[GDP94]	(Gregorini+De Ruiter+Parma+, 1994)
====>	Equivalent to: GDP
Origin	of the Acronym: S = Created by Simbad, the CDS Database
History	of this Acronym: replaced by GDP
Details on Acronym: [GDR2011]
[GDR2011]	(Gouliermis+Dolphin+Robberto+, 2011)
Write:	<<[GDR2011] LHNN NNNNN>>
N:	44649
Object:	* (SIMBAD class: Star)
Note:	HST WFPC2 observations of N=44649 stars in 4 star forming regions in the LMC.
in source:	Magellanic Clouds:LMC = LMC
in source:	LH 60
in source:	LH 63
in source:	LH 72
in source:	LH 88
Ref:	=2011ApJ...738..137G
by	GOULIERMIS D.A. , DOLPHIN A.E., ROBBERTO M., GRUENDL R.A., CHU Y.-H., GENNARO M., HENNING T., ROSA M., DA RIO N., BRANDNER W., ROMANIELLO M., DE MARCHI G., PANAGIA N., ZINNECKER H.
	Astrophys. J., 738, 137 (2011)
	Pre-main-sequence stellar populations across Shapley Constellation III. I. Photometric analysis and identification.
o	Table 3: <[GDR2011] LHNN NNNNN> (Nos LH60 1 to LH60 12511, LH63 1 to LH63 11785, LH72 1 to LH72 9756, LH88 1 to LH88 10597).
=E=	Catalogue in electronic form as J/ApJ/738/137
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GDS
GDS	(Galactic Disk Survey) (Not yet in Simbad)
*****	Avoid the usage of GDS, prefer [HFH2015]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GDS
GDS	(Galactic Disk Survey) (Not yet in Simbad)
*****	Avoid the usage of GDS, prefer [HHR2012]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GDS
GDS	(Gagne+Daniel+Skinner)
Write:	<<GDS JHHMMSS.s+DDMMSS>>
N:	107
Object:	(X) + (Rad) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra and VLA observations of rho Oph cloud: N=87 GDS X-ray sources and N=31 GDS radio sources, 11 are the same GDS source.
in source:	NAME rho Oph Cloud
Ref:	=2004ApJ...613..393G
by	GAGNE M. , SKINNER S.L., DANIEL K.J.
	Astrophys. J., 613, 393-415 (2004)
	Simultaneous Chandra and very large array observations of young stars and protostars in ρ Ophiuchus cloud core A.
o	Objects SKS: this numbering related to the table number in 1995ApJ...438..813S is not used in SIMBAD. So, SKS 1-7 = [SKS95] 162314.6-241237, SKS 3-12 = [SKS95] 162320.8-241803, SKS 1-11 = [SKS95] 162317 .6-241729, etc...
o	Table 1: <GDS JHHMMSS.s+DDMMSS> N=87. Table 3: <GDS JHHMMSS.s+DDMMSS> N=31 (among which 11 are already in Table 1).
=E=	Catalogue in electronic form as J/ApJ/613/393
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GDS
GDS	(Great Observatories Origins Deep Survey)
*****	Avoid the usage of GDS, prefer GOODS
Origin	of the Acronym: L (2004Msngr.118...45V)
Details on Acronym: [GDS2018]
[GDS2018]	(Girard+Dessauges-Zavadsky+Schaerer+, 2018)
Write:	<<[GDS2018] AS1063-NNNN>> <<[GDS2018] AS1063-NNNN 1>> <<[GDS2018] MACS1206-NNNN>> <<[GDS2018] MACS1206-NNNN 1>>
N:	24
Object:	Grav. lensed image of a G (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy)
Note:	VLT KMOS spectroscopic observations of N=24 galaxies in N=2 lensing clusters AS1063 and MACS1206-08, as part of the KMOS LENsing Survey (KLENS).
in source:	ACO S 1063
in source:	MCS J1206.2-0847
Ref:	=2018A&A...613A..72G
by	GIRARD M. , DESSAUGES-ZAVADSKY M., SCHAERER D., CIRASUOLO M., TURNER O.J., CAVA A., RODRIGUEZ-MUNOZ L., RICHARD J., PEREZ-GONZALEZ P.G.
	Astron. Astrophys., 613A, 72-72 (2018)
	KMOS LENsing Survey (KLENS): Morpho-kinematic analysis of star-forming galaxies at z ~ 2.
o	Table 1: <[GDS2018] AS1063-NNNN> N=13 among (Nos 658-1904), <[GDS2018] AS1063-NNNN 1> N=1 (No 606 1), <[GDS2018] MACS1206-NNNN> N=10 among (Nos 415-2372), <[GDS2018] MACS1206-NNNN 1> N=1 (No 1616 1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GDV2009]
[GDV2009]	(Galametz+De Breuck+Vernet+, 2009)
Write:	<<[GDV2009] 7C HHMM+DDMM HzRG>> <<[GDV2009] 7C HHMM+DDMM AGN NN>> <<[GDV2009] 7C HHMM+DDMM NNN>>
N:	2+12+5+129+106
Object:	rG + AGN cand. + G (SIMBAD class: Galaxy)
Note:	Palomar LFC, CFHT WIRCAM and Spitzer IRAC observations of AGN candidates and pBzK* galaxies the fields of 7C 1751+6809 and 7C 1756+6520.
Ref:	=2009A&A...507..131G
by	GALAMETZ A. , DE BREUCK C., VERNET J., STERN D., RETTURA A., MARMO C., OMONT A., ALLEN M., SEYMOUR N.
	Astron. Astrophys., 507, 131-145 (2009)
	Large scale structures around radio galaxies at z ~ 1.5.
o	Tables 3-4: <[GDV2009] 7C HHMM+DDMM HzRG> N=2, <[GDV2009] 7C HHMM+DDMM AGN NN> N=12+5. Tables 5-6: <[GDV2009] 7C HHMM+DDMM NNN> N=129+106.
=E=	Catalogue in electronic form as J/A+A/507/131
Details on Acronym: [GDW2019]
[GDW2019]	(Golovich+Dawson+Wittman+, 2019)
Write:	<<[GDW2019] JDDD.dddddddd+DD.dddddddd A>>
N:	4431
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Subaru SuprimeCam and Keck II DEIMOS observations of N=4431 galaxies in the field of 29 merging galaxy clusters ranging in redshift from z=0.07 to 0.55.
Ref:	=2019ApJS..240...39G
by	GOLOVICH N. , DAWSON W.A., WITTMAN D.M., JEE M.J., BENSON B., LEMAUX B.C., VAN WEEREN R.J., ANDRADE-SANTOS F., SOBRAL D., DE GASPERIN F., BRUGGEN M., BRADAC M., FINNER K., PETER A.
	Astrophys. J., Suppl. Ser., 240, 39-39 (2019)
	Merging cluster collaboration: optical and spectroscopic survey of a radio-selected sample of 29 merging galaxy clusters.
o	Table 7: <[GDW2019] JDDD.dddddddd+DD.dddddddd> N=4418, <[GDW2019] JDDD.dddddddd+DD.dddddddd A> N=13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ge
Ge	(Grebenev+, Einstein)
*****	Avoid the usage of Ge, prefer [GFJ95]
Origin	of the Acronym: L (2002ApJ...576..708S)
Details on Acronym: [GE91]
[GE91]	(Gomez de Castro+Eiroa, 1991)
Write:	<<[GE91] GGD 30 IN>> <<[GE91] GGD 31 IN>> <<[GE91] GGD 31 CN>> <<[GE91] GGD 30 IRS NN>> <<[GE91] GGD 31 IRS>>
N:	3+2+2+16+1
Object:	(IR) in RfN (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=3 point-like sources (Nos I1-I3) in GGD 30. N=2 point-like sources (Nos I1-I2) in GGD 31. N=2 condensations (Nos C1-C2) in GGD 31. Table 2: N=16 IR Sources in GGD 30, format 'GGD 30 IRS NN'. N=1 IR Source in GGD 31, format 'GGD 31 IRS'.
in source:	GGD 30
in source:	GGD 31
Ref:	=1991A&A...241..589G
by	GOMEZ DE CASTRO A.I. , EIROA C.
	Astron. Astrophys., 241, 589-594 (1991)
	An optical and infrared study of the reflection nebulae GGD 30 and GGD 31.
o	Table 1: <[GE91] GGD 30 IN> (Nos I1-I3), <[GE91] GGD 31 IN> (Nos I1-I2), <[GE91] GGD 31 CN> (Nos C1-C2). Table 2: <[GE91] GGD 30 IRS NN> (Nos 1-16), <[GE91] GGD 31 IRS> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GEA97]
[GEA97]	(Girart+Estalella+Anglada+, 1997)= (WHS)
Write:	<<[GEA97] eastern hot spot>> <<[GEA97] western hot spot>>
N:	2
Object:	Hot Spot (SIMBAD class: YSO = Young Stellar Object)
Note:	VLA NH3/H2O and Haystack Observatory 37m telescope 13CO/18CO observations of LDN 723.
in source:	LDN 723
Ref:	=1997ApJ...489..734G
by	GIRART J.M. , ESTALELLA R., ANGLADA G., TORRELLES J.M., HO P.T.P., RODRIGUEZ L.F.
	Astrophys. J., 489, 734-743 (1997)
	The ammonia core in L723: hot spots at the center of the quadrupolar molecular outflow.
o	p. 741 : H2O maser = EQ 191541+190650 in SIMBAD
o	Text: <[GEA97] eastern hot spot> N=1, <[GEA97] western hot spot> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GEC95]
[GEC95]	(Glazebrook+Ellis+Colless+, 1995)= (LDSS-2)
Write:	<<[GEC95] HH.NNN>>
N:	179
Object:	G + * + QSO (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	In the format 'HH' stands for the field R.A., NNN for the zone number N in the field + the number NN within the zone. See also [BAS98], LDSS and LDSS-2
Ref:	=1995MNRAS.273..157G
by	GLAZEBROOK K. , ELLIS R., COLLESS M., BROADHURST T., ALLINGTON-SMITH J., TANVIR N.
	Mon. Not. R. Astron. Soc., 273, 157-168 (1995)
	A faint galaxy redshift survey to B = 24.
o	Table 3, col. (3): <[GEC95] HH.NNN> N=179
=E=	Catalogue in electronic form as J/MNRAS/273/157
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GED2008]
[GED2008]	(GLikman+Eigenbrod+Djorgovski+, 2008)
Write:	<<[GED2008] JHHMMSS.ss+DDMMSS.ss>>
N:	34
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Note:	Search for high-redshift QSOs in the UKIDSS Early Release.
Ref:	=2008AJ....136..954G
by	GLIKMAN E. , EIGENBROD A., DJORGOVSKI S.G., MEYLAN G., THOMPSON D., MAHABAL A., COURBIN F.
	Astron. J., 136, 954-962 (2008)
	An exploratory search for z ≳ 6 quasars in the UKIDSS early data release.
o	Table 1: <[GED2008] JHHMMSS.ss+DDMMSS.ss> N=34.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GEH2000]
[GEH2000]	(Girart+Estalella+Ho+, 2000)= (JMG99) (Not yet in Simbad)
Write:	<<[GEH2000] GN>>
N:	2
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Note:	N=2 clumps in the star-forming region [MLS88] G. See [MLS88].
in source:	[MLS88] G
Ref:	=2000ApJ...539..763G
by	GIRART J.M. , ESTALELLA R., HO P.T.P., RUDOLPH A.L.
	Astrophys. J., 539, 763-774 (2000)
	A multitransition HCO^+ study in NGC 2264G: anomalous emission of the J=1⟶0 line.
o	Fig.1: <[GEH2000] GN> (Nos G1-G2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GEL
GEL	(Gomez de Castro+Eiroa+Lenzen)
Write:	<<GEL NN>>
N:	18
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Rem:	Identif. charts
in source:	NAME Serpens Cloud
Ref:	=1988A&A...201..299G
by	GOMEZ DE CASTRO A.I. , EIROA C., LENZEN R.
	Astron. Astrophys., 201, 299-310 (1988)
	Observational evidence for the influence of the magnetic field on star formation in the Serpens molecular cloud.
o	Table 2: <GEL NN> N=18
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Gem
Gem	(Gemini)
*****	Avoid the usage of Gem, prefer [CSS95]
Origin	of the Acronym: L (2003ARA&A..41...57L)
Details on Acronym: Gem
Gem	(Gemini OB 1)
*****	Avoid the usage of Gem, prefer Glazar
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Gem
Gem	(Gemini)
*****	Avoid the usage of Gem, prefer [MWC53]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Geminga
Geminga	(source in Gem)
N:	1
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Geminga was first noticed as a strong gamma-ray source.
in source:	NAME GEM
Ref:	=1977ApJ...213..252T
by	THOMPSON D.J. , FICHTEL C.E., HARTMAN R.C., KNIFFEN D.A., LAMB R.C.
	Astrophys. J., 213, 252-262 (1977)
	Final SAS-2 γ-ray results on sources in the galactic anticenter region.
o	<NAME GEMINGA>
Details on Acronym: GEMS
GEMS	(Group Evolution Multiwavelength Study)
*****	Avoid the usage of GEMS, prefer [BFK2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GEMS
GEMS	(Group Evolution Multiwavelength Study)
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
in source:	NAME NGC 1332 GROUP
in source:	NAME NGC 1808 GROUP
in source:	NAME NGC 3923 GROUP
in source:	NAME NGC 5044 GROUP
in source:	NAME NGC 7144 GROUP
in source:	HCG 90
Ref:	=2008MNRAS.384..305K
by	KERN K.M. , KILBORN V.A., FORBES D.A., KORIBALSKI B.
	Mon. Not. R. Astron. Soc., 384, 305-315 (2008)
	HI mapping of galaxies in six Group Evolution Multiwavelength Study groups.
o	Table 2: <[BFK2006] GEMS-N1332-NN>, <[BFK2006] GEMS-N1808-NN>, <[BFK2006] GEMS-N3923-NN>, <[BFK2006] GEMS-N5044-NN>, <[BFK2006] GEMS-N7144-NNA>, <[BFK2006] GEMS-HCG90-NNA>, N=19.
*****	Avoid the usage of GEMS, prefer [KKF2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GEMS
GEMS	(Galaxy Evolution from Morphology and SEDs)
Write:	<<GEMS JHHMMSS.ss+DDMMSS.sA>>
N:	41495
Object:	G (SIMBAD class: Galaxy)
Note:	The Galaxy Evolution from Morphology and SEDs HST survey is described in 2004ApJS..152..163R. In 2006ApJ...640..241B, GEMS is used in combination with the COMBO-17 survey and letters A and B at the end of the format stands for subcomponents when the system was not resolved into two separate galaxies by COMBO-17. Complete catalog in 2007ApJS..172..615H.
Ref:	=2006ApJ...640..241B
by	BELL E.F. , NAAB T., McINTOSH D.H., SOMERVILLE R.S., CALDWELL J.A.R., BARDEN M., WOLF C., RIX H.-W., BECKWITH S.V., BORCH A., HAUSSLER B., HEYMANS C., JAHNKE K., JOGEE S., KOPOSOV S., MEISENHEIMER K., PENG C.Y., SANCHEZ S.F., WISOTZKI L.
	Astrophys. J., 640, 241-251 (2006)
	Dry mergers in GEMS: the dynamical evolution of massive early-type galaxies.
o	Table 1: <GEMS JHHMMSS.ss+DDMMSS.s> N=32.
Ref:	=2007ApJS..172..615H
by	HAUSSLER B. , McINTOSH D.H., BARDEN M., BELL E.F., RIX H.-W., BORCH A., BECKWITH S.V.W., CALDWELL J.A.R., HEYMANS C., JAHNKE K., JOGEE S., KOPOSOV S.E., MEISENHEIMER K., SANCHEZ S.F., SOMERVILLE R.S., WISOTZKI L., WOLF C.
	Astrophys. J., Suppl. Ser., 172, 615-633 (2007)
	GEMS: galaxy fitting catalogs and testing parametric galaxy fitting codes: GALFIT and GIM2D.
o	Table 9: <GEMS JHHMMSS.ss+DDMMSS.s> N=41495.
=E=	Catalogue in electronic form as J/ApJS/172/615
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GemWD
GemWD	(Davis+Richer+Rich+, 2009)
*****	Avoid the usage of GemWD, prefer [DRR2009]
Origin	of the Acronym: A (2009ApJ...705..408K)
Details on Acronym: GEN
GEN	(Genzel)
*****	Avoid the usage of GEN, prefer [RGH2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GEN#
GEN#	(Geneva identification system)
Write:	<<GEN# +N.NNNNNNNNA>>
Object:	* (SIMBAD class: Star)
Note:	Geneva Identification system: in SIMBAD only. Similar to LID
Details on Acronym: [GEN2002]
[GEN2002]	(Greenhill+Ellingsen+Norris+, 2002)
Write:	<<[GEN2002] H2O HHMMm+DDMM>>
N:	1
Object:	H2O Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	Discovery of a maser in the galaxy IRAS F01063-8034.
in source:	IRAS F01063-8034
Ref:	=2002ApJ...565..836G
by	GREENHILL L.J. , ELLINGSEN S.P., NORRIS R.P., McGREGOR P.J., GOUGH R.G., SINCLAIR M.W., RAYNER D.P., PHILLIPS C.J., HERRNSTEIN J.R., MORAN J.M.
	Astrophys. J., 565, 836-848 (2002)
	A search for H_{2}O maser emission in southern active galactic nuclei and star-forming galaxies: discovery of a maser in the edge-on galaxy IRAS F01063-8034.
o	<[GEN2002] H2O HHMMm+DDMM> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GEO97]
[GEO97]	(Genzel+Eckart+Ott+, 1997)= (W)
Write:	<<[GEO97] WNN>>
N:	18
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Stars are mostly West and South-West of Sgr A*. See also [EG97], [GKM98], [PGM2006], [RGH2007].
in source:	NAME Gal Center
Ref:	=1997MNRAS.291..219G
by	GENZEL R. , ECKART A., OTT T., EISENHAUER F.
	Mon. Not. R. Astron. Soc., 291, 219-234 (1997)
	On the nature of the dark mass in the centre of the Milky Way.
o	Table 1: sources S1 to S11 = [EG97] SNN
o	Fig.1: <[EG97] S12> added. Table 1: <GCIRS 29S1>, <GCIRS 29S2> new. Table 1: <[GEO97] WNN> (Nos W1-W18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Gershberg
Gershberg	(List of Gersbergh)
Write:	<<Gershberg NN>>
N:	78
Object:	Flare * (SIMBAD class: Eruptive* = Eruptive Variable)
Note:	Table 2: list of 78 * from Gershberg R.E., 1978, Low Mass Flaring Stars (Moscow: Nauka)
Ref:	=1989ApJ...343..400M
by	MULLAN D.J. , STENCEL R.E., BACKMAN D.E.
	Astrophys. J., 343, 400-408 (1989)
	Far-infrared properties of flare stars and dM stars.
o	Table 2: <Gershberg NN> N=78
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GES
GES	(Gaia-ESO Survey)
Write:	<<GES JHHMMSSss+DDMMSSs>> <<GES HHMMSSss+DDMMSSs>> (not recognised by Simbad, but found in literature)
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Coordinate-based identification of objects from the Gaia-ESO Survey. More information on the suvey at http://www.gaia-eso.eu/ The first data release is available at the ESO Science Archive (http://archive.eso.org/wdb/wdb/adp/phase3_spectral/form?phase3_collection=GaiaESO&release_tag=1). Only the first reference citing GES objects is given here.
Ref:	=2014A&A...561A..94D
by	DONATI P. , CANTAT GAUDIN T., BRAGAGLIA A., FRIEL E., MAGRINI L., SMILJANIC R., VALLENARI A., TOSI M., SORDO R., TAUTVAISIENE G., BLANCO-CUARESMA S., COSTADO M.T., GEISLER D., KLUTSCH A., MOWLAVI N., MUNOZ C., SAN ROMAN I., ZAGGIA S., GILMORE G., RANDICH S., BENSBY T., FLACCOMIO E., KOPOSOV S.E., KORN A.J., PANCINO E., RECIO-BLANCO A., FRANCIOSINI E., DE LAVERNY P., LEWIS J., MORBIDELLI L., PRISINZANO L., SACCO G., WORLEY C.C., HOURIHANE A., JOFRE P., LARDO C., MAIORCA E.
	Astron. Astrophys., 561A, 94-94 (2014)
	The Gaia-ESO Survey: reevaluation of the parameters of the open cluster Trumpler 20 using photometry and spectroscopy.
o	Table 3: <GES JHHMMSSss+DDMMSSs> N=1370.
=E=	Catalogue in electronic form as J/A+A/561/A94
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GES2010]
[GES2010]	(Grillo+Eichner+Seitz+, 2010)
Write:	<<[GES2010] SDSS J1538+5817 AN>>
N:	6
Object:	Grav. lensed image of a G (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2/ACS photometry and NOT ALFOSC spectroscopy of two systems of multiple images of the gravitational lens system SLACS SDSS J1538+5817: a double (D1-D2) and a quad (Q1-Q4).
in source:	SLACS SDSS J1538+5817
Ref:	=2010ApJ...710..372G
by	GRILLO C. , EICHNER T., SEITZ S., BENDER R., LOMBARDI M., GOBAT R., BAUER A.
	Astrophys. J., 710, 372-384 (2010)
	Golden gravitational lensing systems from the Sloan lens ACS survey. I. SDSS J1538+5817: one lens for two sources.
o	Fig. 7, Table 2: <[GES2010] SDSS J1538+5817 AN> (Nos D1-D2, Q1-Q4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GES82]
[GES82]	(Goss+Ekers+Skellern+, 1982)
Write:	<<[GES82] HHMM+DDd>> <<[GES82] a>>
N:	4+6
Object:	(Rad) + G (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=4 Radio-sources in the field of PKS 2006-56. Table 2: N=6 galaxies in the field of PKS 2006-56. Plate 2: map.
Ref:	=1982MNRAS.198..259G
by	GOSS W.M. , EKERS R.D., SKELLERN D.J., SMITH R.M.
	Mon. Not. R. Astron. Soc., 198, 259-264 (1982)
	Radio emission from the 2006-56 region.
o	Table 1: <[GES82] HHMM-DDd> N=4. Table 2: <[GES82] a> (Nos a-f).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GeV
GeV	(Giga electron Volt)
Write:	<<GeV JHHMM+DDMM>>
N:	57
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	Observations with the EGRET instrument on the Compton Gamma Ray Observatory. See also TeV.
Ref:	=1997ApJ...488..872L
by	LAMB R.C. , MACOMB D.J.
	Astrophys. J., 488, 872-880 (1997)
	Point sources of GeV γ rays.
o	Tables 1, 2, 3: <GeV JHHMM+DDMM> N=57
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GEX2022]
[GEX2022]	(Gomez-Guijarro+Elbaz+Xiao+, 2022)
Write:	<<[GEX2022] A2GSNNN>>
N:	104
Object:	G (SIMBAD class: Galaxy)
Note:	ALMA 1.1mm observations of N=104 galaxies in the GOODS South fields, as part of the GOODS-ALMA 1.1mm galaxy survey. Nos A2GS1-A2GS44: Main catalog of 100% pure sources Nos A2GS45-A2GS88: Supplementary catalog of prior-based selected sources Nos A2GS89-A2GS104: Uncertain sources See also [FEB2018].
in source:	NAME GOODS South Field
Ref:	=2022A&A...658A..43G
by	GOMEZ-GUIJARRO C. , ELBAZ D., XIAO M., BETHERMIN M., FRANCO M., MAGNELLI B., DADDI E., DICKINSON M., DEMARCO R., INAMI H., RUJOPAKARN W., MAGDIS G.E., SHU X., CHARY R., ZHOU L., ALEXANDER D.M., BOURNAUD F., CIESLA L., FERGUSON H.C., FINKELSTEIN S.L., GIAVALISCO M., IONO D., JUNEAU S., KARTALTEPE J.S., LAGACHE G., LE FLOC'H E., LEITON R., LIN L., MOTOHARA K., MULLANEY J., OKUMURA K., PANNELLA M., PAPOVICH C., POPE A., SARGENT M.T., SILVERMAN J.D., TREISTER E., WANG T.
	Astron. Astrophys., 658A, 43-43 (2022)
	GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies.
o	Tables 2-3, B.1: <[GEX2022] A2GSNNN> (Nos 1-104).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GF
GF	(Globular Filament)
Write:	<<GF NN>> <<GF NNA>> <<GF NNAN>> <<GF NNAa>> <<GF NNANa>>
N:	23+90+109+6+32
Object:	GF (SIMBAD class: ISM = Interstellar Medium Object)
Note:	Table 3: N=23 Globular Filaments, (Nos 1-23). Figs 1-20: 3 hierarchies of condensations in each filament are considered: hierarchy 1 is denoted by a capital letter, format 'NNA', hierarchy 2 is denoted by a number, format 'NNAN', hierarchy 3 is denoted by a lowercase letter, format 'NNANa', Thus the name of an individual condensation might be 'GF 3A1b', which is the second sub-subfragment (b) inside the first subfragment (1) inside the first fragment (A) of the globular filament 3. Identif. charts
Ref:	=1979ApJS...41...87S
by	SCHNEIDER S. , ELMEGREEN B.G.
	Astrophys. J., Suppl. Ser., 41, 87-95 (1979)
	A catalog of dark globular filaments.
o	Table 3: <GF NN> (Nos 1-23). Plates 1-20: <GF NNA> N=90, <GF NNAN> N=109, <GF NNAa> N=6, <GF NNANa> N=32.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GF
GF	(Glass+Feast)
*****	Avoid the usage of GF, prefer [GF73]
Origin	of the Acronym: L (1997ApJ...489..254C)
Details on Acronym: GF 9
GF 9	(Globular Filament 9)
*****	Avoid the usage of GF 9, prefer [PB2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GF2000]
[GF2000]	(Giovannini+Feretti, 2000)
Write:	<<[GF2000] ACO 85 A>> <<[GF2000] ACO 401 A>>
N:	5+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA observations of the halos and relics of 2 clusters.
in source:	ACO 85
in source:	ACO 401
Ref:	=2000NewA....5..335G
by	GIOVANNINI G. , FERETTI L.
	New Astronomy, 5, 335-347 (2000)
	Halo and relic sources in clusters of galaxies.
o	Fig.1: <[GF2000] ACO 85 A> (Nos A-D, R). Fig.11: <[GF2000] ACO 401 A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GF2001]
[GF2001]	(Gerardy+Fesen, 2001)= (FMK) = (QSF) (Not yet in Simbad)
Write:	<<[GF2001] FMK N>> <<[GF2001] QSF N>>
N:	5+3
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Note:	N=5 Fast-Moving Knots (FMK) and N=3 Quasi-Stellar Floculi (QSF) in NIR observations of Cas A. See also [HF96].
in source:	NAME Cas A
Ref:	=2001AJ....121.2781G
by	GERARDY C.L. , FESEN R.A.
	Astron. J., 121, 2781-2791 (2001)
	Near-infrared spectroscopy of the Cassiopeia A and Kepler supernova remnants.
o	Fig.1, Table 1: <[GF2001] FMK N> (Nos 1-5), <[GF2001] QSF N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GF2002]
[GF2002]	(Graham+Fassett, 2002)
Write:	<<[GF2002] Blue NN>> <<[GF2002] DF 6-NN>>
N:	31+13
Object:	* (SIMBAD class: Star)
Note:	Las Campanas observations. N=31 blue stars in the inner jet of Cen A. N=13 stars in the [DV78] DF 6 stellar association.
in source:	Cen A = NGC 5128
Ref:	=2002ApJ...575..712G
by	GRAHAM J.A. , FASSETT C.I.
	Astrophys. J., 575, 712-720 (2002)
	Star formation associated with the X-ray jet in Centaurus A.
o	Knots 'A' = 'BGLO Cen A Knot A'.
o	Table 1, Fig.4: <[GF2002] Blue NN> (Nos 1-31). Table 2, Fig.7: <[GF2002] DF 6-NN> (Nos 6-1 to 6-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GF73]
[GF73]	(Glass+Feast, 1973)= (GF)
Write:	<<[GF73] A>>
N:	2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=2 stars (Nos A-B). Star 'B' is found later in the literature as 'GF star' = V* V2116 Oph. Map in Fig.1.
Ref:	=1973NPhS..245...39G
by	GLASS I.S. , FEAST M.W.
	Nature, Physical Science, 245, 39-39 (1973)
	Peculiar object near X2+5.
o	X2+5 = GX 2+5
o	Fig.1: <[GF73] A> (Nos A-B)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GF92]
[GF92]	(Geisler +Friel, 1992) (Not yet in Simbad)
Write:	<<[GF92] NNNN>>
N:	314
Object:	G or K Giant (SIMBAD class: Star)
Note:	N = 3539 in the total calibrated list.
Ref:	=1992AJ....104..128G
by	GEISLER D. , FRIEL E.D.
	Astron. J., 104, 128-143 (1992)
	The metallicity distribution of G and K giants in Baade's window.
o	<[GF92] NNNN> N=314
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFB2000]
[GFB2000]	(Garmire+Feigelson+Broos+, 2000)
Write:	<<[GFB2000] ONC NNN>> <<[GFB2000] BN NN>>
N:	973+27
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS-I observations. X-ray emitting young stars in the Orion Nebula region and the BN object region. See also CXOONC.
in source:	NAME ONC
in source:	NAME BN Object
Ref:	=2000AJ....120.1426G
by	GARMIRE G. , FEIGELSON E.D., BROOS P., HILLENBRAND L.A., PRAVDO S.H., TOWNSLEY L., TSUBOI Y.
	Astron. J., 120, 1426-1435 (2000)
	Chandra X-ray observatory study of the Orion nebula cluster and BN/KL region.
o	Infrared source n = LBLS n, source radio D = GMR D
o	Table 1: <[GFB2000] ONC NNN> (Nos 1-973) = <CXOONC JHHMMSS.s+DDMMSS> N=973. Table 2: <[GFB2000] BN NN> (Nos 1-27) = <CXOONC JHHMMSS.s+DDMMSS> N=27.
=E=	Catalogue in electronic form as J/AJ/120/1426
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFC2006]
[GFC2006]	(Gandhi+Fabian+Crawford, 2006)
Write:	<<[GFC2006] N>>
N:	4
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	WHT i band photometry and NOT optical spectroscopy of 4C +39.29 to search for the optical counterpart.
Ref:	=2006MNRAS.369.1566G
by	GANDHI P. , FABIAN A.C., CRAWFORD C.S.
	Mon. Not. R. Astron. Soc., 369, 1566-1576 (2006)
	4C +39.29 - extended emission around a powerful type 2 quasar.
o	Fig.1: <[GFC2006] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GFC2012
GFC2012	(Galvin, Filipovic, Crawford published in 2012) (Not yet in Simbad)
Write:	<<GFC2012 JHHMMSS.s+DDMMSS>>
N:	72
Object:	Radio continuum (SIMBAD class: Radio = Radio Source)
Note:	Paper accepted for publication in Astrophysics and Space Science. Title "Radio-Continuum study of the Nearby Sculptor Group Galaxies. Part 1: NGC300 at lambda=20cm", Authors: T. J. Galvin, M. Filipovic, E. Crawford et. al.
Auth.:	Timothy Galvin University of Western Sydney
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [GFC96]
[GFC96]	(Garcia-Barreto+Franco+Carrillo, 1996) (Not yet in Simbad)
Write:	<<[GFC96] Na>>
N:	10
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
in source:	NGC 3367
Ref:	=1996ApJ...469..138G
by	GARCIA-BARRETO J.A. , FRANCO J., CARRILLO R.
	Astrophys. J., 469, 138-146 (1996)
	On the origin of the southwest Hα regions of the spiral galaxy NGC 3367.
o	Table 2: <[GFC96] Na> (Nos 1-6, 7a-7b, 8-9)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFF2005]
[GFF2005]	(Gorosabel+Fynbo+Fruchter+, 2005)
Write:	<<[GFF2005] A>>
N:	10
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	NOT observations of the GRB020305 field. N=10 secondary standard stars.
Ref:	=2005A&A...437..411G
by	GOROSABEL J. , FYNBO J.P.U., FRUCHTER A., LEVAN A., HJORTH J., NUGENT P., CASTRO-TIRADO A.J., CASTRO CERON J.M., RHOADS J., BERSIER D., BURUD I.
	Astron. Astrophys., 437, 411-418 (2005)
	A possible bright blue supernova in the afterglow of GRB 020305.
o	Fig.1, Table 1: <[GFF2005] A> (Nos A-J).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFF2012]
[GFF2012]	(Govoni+Ferrari+Feretti+, 2012)
Write:	<<[GFF2012] ANNNN A>> <<[GFF2012] CL1446+26 A>>
N:	17 (SIMBAD class: Radio = Radio Source)
Note:	VLA 1.4 GHz observations of N=4 galaxy clusters.
in source:	ACO 800
in source:	ACO 910
in source:	ACO 1550
in source:	ClG 1446+26
Ref:	=2012A&A...545A..74G
by	GOVONI F. , FERRARI C., FERETTI L., VACCA V., MURGIA M., GIOVANNINI G., PERLEY R., BENOIST C.
	Astron. Astrophys., 545A, 74-74 (2012)
	Detection of diffuse radio emission in the galaxy clusters A800, A910, A1550, and CL 1446+26.
o	Table 2: <[GFF2012] ANNNN A> <[GFF2012] CL1446+26 A> N=17 (Nos [GFF2012] A800 A-B, [GFF2012] A910 A-F, [GFF2012] A1550 A-C, [GFF2012] CL1446+26 A-F)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFF99]
[GFF99]	(Graham+Ferrarese+Freedman+, 1999)
Write:	<<[GFF99] N-NN>> <<[GFF99] CNN>> <<[GFF99] VNN>>
N:	30+24+11
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	HST observations of NGC 4548. Table 3: Bright stars in chips 1 to 4, N=30. Table 5: (Nos C1-C24), N=24 Cepheids. Table 8: (Nos V1-V11), N=11 V*. See also: [FHM94], [HST94], [KIF96], [FFH96], [SHM96], [GPF97], [RMM97], [PSF98], [FBK98], [HHH98], [TFS98], [GHS99], [KIS99], [SHF99], [MHS99], [SFK99], [PKB99], [GSF2000], [MHS2000]
in source:	NGC 4548
Ref:	=1999ApJ...516..626G
by	GRAHAM J.A. , FERRARESE L., FREEDMAN W.L., KENNICUTT R.C.Jr, MOULD J.R., SAHA A., STETSON P.B., MADORE B.F., BRESOLIN F., FORD H.C., GIBSON B.K., HAN M., HOESSEL J.G., HUCHRA J., HUGHES S.M., ILLINGWORTH G.D., KELSON D.D., MACRI L., PHELPS R., SAKAI S., SILBERMANN N.A., TURNER A.
	Astrophys. J., 516, 626-646 (1999)
	The Hubble space telescope key project on the extragalactic distance scale. XX. The discovery of cepheids in the Virgo cluster galaxy NGC 4548.
o	Table 3: <[GFF99] N-NN> N=30. Table 5: <[GFF99] CNN> (Nos C1-C24). Table 8: <[GFF99] VNN> (Nos V1-V11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GFG
GFG	(Giardino+Favata+G?)
*****	Avoid the usage of GFG, prefer [GFM2007]
Origin	of the Acronym: L (2007ApJ...669..493W)
Details on Acronym: [GFG2007]
[GFG2007]	(Getman+Feigelson Garmire+, 2007)
Write:	<<[GFG2007] NNN>>
N:	117
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of IC 1396N.
in source:	IC 1696:IC 1396N = IC 1396N
Ref:	=2007ApJ...654..316G
by	GETMAN K.V. , FEIGELSON E.D., GARMIRE G., BROOS P., WANG J.
	Astrophys. J., 654, 316-337 (2007)
	X-ray study of triggered star formation and protostars in IC 1396N.
o	Table 5: Objects CRBR NN are not identified (format CRBR MMSS.s-MMSS in SIMBAD).
o	Table 1: <[GFG2007] NNN> (Nos 1-117).
=E=	Catalogue in electronic form as J/ApJ/654/316
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFG2013]
[GFG2013]	(Guaita+Francke+Gawiser+, 2013)= ([GFG2013a])
Write:	<<[GFG2013] AGNNN>> <<[GFG2013] BzK25>> <<[GFG2013] BXNN>> <<[GFG2013] LAE27>> <<[GFG2013] zNLAEN>> <<[GFG2013] DBNN>> <<[GFG2013] LBG11>>
N:	17
Object:	Star-forming G (SIMBAD class: Galaxy)
Note:	Magellan MMIRS NIR spectroscopy of N=17 sources in three MUSYC fields.
Ref:	=2013A&A...551A..93G
by	GUAITA L. , FRANCKE H., GAWISER E., BAUER F.E., HAYES M., OESTLIN G., PADILLA N.
	Astron. Astrophys., 551A, 93-93 (2013)
	Magellan/MMIRS near-infrared multi-object spectroscopy of nebular emission from star-forming galaxies at 2 < z < 3.
o	Table 3: <[GFG2013] AGNNN> (Nos AGN5, AGN26), <[GFG2013] BzK25> N=1, <[GFG2013] BXNN> N=6 among (Nos 1-16), <[GFG2013] LAE27> N=1, <[GFG2013] zNLAEN> (Nos z2LAE2-3, z3LAE2), <[GFG2013] DBNN> (Nos 8,12,22), <[GFG2013] LBG11> N=1.
=E=	Catalogue in electronic form as <J/A+A/551/A93/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFG2013a]
[GFG2013a]	(Guaita+Francke+Gawiser+, 2013)
*****	Avoid the usage of [GFG2013a], prefer [GFG2013]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFG2013b]
[GFG2013b]	(Guo+Ferguson+Giavalisco+, 2013)
Write:	<<[GFG2013b] NNNNN>>
N:	34930
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	UV to mid-infrared multi-wavelength catalog of N=34930 F160W-selected sources in the CANDELS GOODS-South field, as part of the CANDELS survey. See also CANDELS GDS F160W.
in source:	NAME GOODS South Field
Ref:	=2013ApJS..207...24G
by	GUO Y. , FERGUSON H.C., GIAVALISCO M., BARRO G., WILLNER S.P., ASHBY M.L.N., DAHLEN T., DONLEY J.L., FABER S.M., FONTANA A., GALAMETZ A., GRAZIAN A., HUANG K.-H., KOCEVSKI D.D., KOEKEMOER A.M., KOO D.C., McGRATH E.J., PETH M., SALVATO M., WUYTS S., CASTELLANO M., COORAY A.R., DICKINSON M.E., DUNLOP J.S., FAZIO G.G., GARDNER J.P., GAWISER E., GROGIN N.A., HATHI N.P., HSU L.-T., LEE K.-S., LUCAS R.A., MOBASHER B., NANDRA K., NEWMAN J.A., VAN DER WEL A.
	Astrophys. J., Suppl. Ser., 207, 24 (2013)
	CANDELS multi-wavelength catalogs: source detection and photometry in the GOODS-south field.
o	catalog.dat: <[GFG2013b] NNNNN> (Nos 1-34930) = <CANDELS GDS F160W JHHMMSS.ss+DDMMSS.s> N=34930.
=E=	Catalogue in electronic form as J/ApJS/207/24
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFG97]
[GFG97]	(Green+Frail+Goss+, 1997)
Write:	<<[GFG97] HHMMSS.ss+DDMMSS.s>> <<[GFG97] HHMMSS.s+DDMMSS>>
N:	5
Object:	OH Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	N=5 OH masers towards 4 SNR.
in source:	SNR G016.7+00.1
in source:	Kes 69
in source:	IRAS 18379-0500
in source:	W 51:W 51C = W 51C
Ref:	=1997AJ....114.2058G
by	GREEN A.J. , FRAIL D.A., GOSS W.M., OTRUPCEK R.
	Astron. J., 114, 2058-2067 (1997)
	Continuation of a survey of OH (1720 MHz) maser emission towards supernova remnants.
o	Table 2: <[GFG97] HHMMSS.ss+DDMMSS.s>, <[GFG97] HHMMSS.s+DDMMSS>, N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFH2002]
[GFH2002]	(Gorosabel+Fynbo+Hjorth+, 2002)
Write:	<<[GFH2002] N>> <<[GFH2002] JHHMMSS.ss+DDMMSS.s>>
N:	6+1
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=6 secondary standards in the field of GRB 001011. N=1 Host galaxy.
Ref:	=2002A&A...384...11G
by	GOROSABEL J. , FYNBO J.U., HJORTH J., WOLF C., ANDERSEN M.I., PEDERSEN H., CHRISTENSEN L., JENSEN B.L., MOLLER P., AFONSO J., TREYER M.A., MALLEN-ORNELAS G., CASTRO-TIRADO A.J., FRUCHTER A., GREINER J., PIAN E., VREESWIJK P.M., FRONTERA F., KAPER L., KLOSE S., KOUVELIOTOU C., MASETTI N., PALAZZI E., ROL E., SALAMANCA I., TANVIR N., WIJERS R.A.M.J., VAN DEN HEUVEL E.
	Astron. Astrophys., 384, 11-23 (2002)
	Strategies for prompt searches for GRB afterglows: The discovery of the GRB 001011 optical/near-infrared counterpart using colour-colour selection.
o	Fig.1, Table 2: <[GFH2002] N> (Nos 1-6). Text: <[GFH2002] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFJ95]
[GFJ95]	(Grebenev+Forman+Jones+, 1995)= (Gp) = (Ge)
Write:	<<[GFJ95] rNN>> <<[GFJ95] eNN>>
N:	31+28
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Table 1: X-ray observations with the ROSAT PSPC, (Nos r1-r31). Table 3: X-ray observations with the HRI aboard Einstein, (Nos e1-e28).
in source:	ACO 1367
Ref:	=1995ApJ...445..607G
by	GREBENEV S.A. , FORMAN W., JONES C., MURRAY S.
	Astrophys. J., 445, 607-623 (1995)
	Wavelet transform analysis of the small-scale X-ray structure of the cluster Abell 1367.
o	Tables 1, 2: <[GFJ95] rNN> (Nos r1-r31), Table 3: <[GFJ95] eNN> (Nos e1-e28)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFK2014]
[GFK2014]	(Gozaliasl+Finoguenov+Khosroshahi+, 2014)
Write:	<<[GFK2014] NNNNNN>>
N:	128
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	XMM-Newton CFHTLS W1 field observations of N=128 X-ray galaxy groups from XMM-Newton and CFTHLS observations in the CFTHLS W1 field. Use of VVDS archival data.
Ref:	=2014A&A...566A.140G
by	GOZALIASL G. , FINOGUENOV A., KHOSROSHAHI H.G., MIRKAZEMI M., SALVATO M., JASSUR D.M.Z., ERFANIANFAR G., POPESSO P., TANAKA M., LERCHSTER M., KNEIB J.P., McCRACKEN H.J., MELLIER Y., EGAMI E., PEREIRA M.J., BRIMIOULLE F., ERBEN T., SEITZ S.
	Astron. Astrophys., 566A, 140-140 (2014)
	Mining the gap: evolution of the magnitude gap in X-ray galaxy groups from the 3-square-° XMM coverage of CFHTLS.
o	Table 1: <[GFK2014] NNNNNN> N=128 among (Nos 100010 to 103340) = <XMMU JHHMMSS.s+DDMMSS> N=128.
=E=	Catalogue in electronic form as J/A+A/566/A140
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFL2008]
[GFL2008]	(Getman+Feigelson+Lawson+, 2008)
Write:	<<[GFL2008] R NN>>
N:	93+14+9+12
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of the globule CG 12.
in source:	CG 12
Ref:	=2008ApJ...673..331G
by	GETMAN K.V. , FEIGELSON E.D., LAWSON W.A., BROOS P.S., GARMIRE G.P.
	Astrophys. J., 673, 331-353 (2008)
	The stellar population and origin of the mysterious high-latitude star-forming cloud CG 12.
o	Table 2: <[GFL2008] R NN> N=93+14+9+12.
=E=	Catalogue in electronic form as J/ApJ/673/331
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFL2009]
[GFL2009]	(Graham+Fruchter+Levan+, 2009)= ([GFL2009a])
Write:	<<[GFL2009] GRB 070714B Host Galaxy>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Note:	Gemini GMOS and NIRI, and Keck II NIRSPEC observations of the host galaxy of GRB 070714B.
Ref:	=2009ApJ...698.1620G
by	GRAHAM J.F. , FRUCHTER A.S., LEVAN A.J., MELANDRI A., KEWLEY L.J., LEVESQUE E.M., NYSEWANDER M., TANVIR N.R., DAHLEN T., BERSIER D., WIERSEMA K., BONFIELD D.G., MARTINEZ-SANSIGRE A.
	Astrophys. J., 698, 1620-1629 (2009)
	GRB 070714B–Discovery of the highest spectroscopically confirmed short burst redshift.
o	<[GFL2009] GRB 070714B Host Galaxy> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFL2009a]
[GFL2009a]	(Graham+Fruchter+Levan+, 2009)
*****	Avoid the usage of [GFL2009a], prefer [GFL2009]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFL2009b]
[GFL2009b]	(Getman+Feigelson+Luhman+, 2009)
Write:	<<[GFL2009b] NNN>>
N:	224
Object:	Poss. PMS* (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC observations of Cep B and Cep OB3b.
in source:	NAME Cep B
in source:	NAME Ass Cep OB 3b
Ref:	=2009ApJ...699.1454G
by	GETMAN K.V. , FEIGELSON E.D., LUHMAN K.L., SICILIA-AGUILAR A., WANG J., GARMIRE G.P.
	Astrophys. J., 699, 1454-1472 (2009)
	Protoplanetary disk evolution around the triggered star-forming region Cepheus B.
o	Table 3: <[GFL2009b] NNN> (Nos 1-224).
=E=	Catalogue in electronic form as <J/ApJ/699/1454/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFM2004]
[GFM2004]	(Garay+Faundez+Mardones+, 2004)= ([GFM2004a]) = (SIMBA)
Write:	<<[GFM2004] GLLL.lll+B.bbb>>
N:	4
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Observations with SEST at La Silla, using SEST Imaging Bolometer Array (SIMBA). N=4 strong 1.2mm sources.
Ref:	=2004ApJ...610..313G
by	GARAY G. , FAUNDEZ S., MARDONES D., BRONFMAN L., CHINI R., NYMAN L.-A.
	Astrophys. J., 610, 313-319 (2004)
	Discovery of four new massive and dense cold cores.
o	Table 2: <[GFM2004] GLLL.lll+B.bbb> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFM2004a]
[GFM2004a]	(Garay+Faundez+Mardones+, 2004)
*****	Avoid the usage of [GFM2004a], prefer [GFM2004]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFM2004b]
[GFM2004b]	(Giardino+Favata+Micela+, 2004)
Write:	<<[GFM2004b] S106 NN>> <<[GFM2004b] S106 South N>>
N:	87+6
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of Sh 2-106 region.
in source:	SH 2-106
Ref:	=2004A&A...424..965G
by	GIARDINO G. , FAVATA F., MICELA G.
	Astron. Astrophys., 424, 965-978 (2004)
	Chandra observations of the massive star-forming region S106 X-ray emission from the embedded massive protostellar object IRS 4.
o	Table 1: <[GFM2004b] S106 NN> (Nos 1-87). Table 2: <[GFM2004b] S106 South N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFM2006]
[GFM2006]	(Gallo+Fender+Miller-Jones+, 2006)
Write:	<<[GFM2006] 0620-00 WW>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 8.46GHz observations of the field of 1A 0620-00: N=2 new sources are found.
Ref:	=2006MNRAS.370.1351G
by	GALLO E. , FENDER R.P., MILLER-JONES J.C.A., MERLONI A., JONKER P.G., HEINZ S., MACCARONE T.J., VAN DER KLIS M.
	Mon. Not. R. Astron. Soc., 370, 1351-1360 (2006)
	A radio-emitting outflow in the quiescent state of A0620-00: implications for modelling low-luminosity black hole binaries.
o	Fig.2, Table 2: <[GFM2006] 0620-00 WW> (Nos N, NE).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFM2007]
[GFM2007]	(Giardino+Favata+Micela+, 2007)= (GFG)
Write:	<<[GFM2007] NN>>
N:	85
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations to search for X-ray emission in YSO in the Serpens star-forming region.
in source:	NAME Serpens Region
Ref:	=2007A&A...463..275G
by	GIARDINO G. , FAVATA F., MICELA G., SCIORTINO S., WINSTON E.
	Astron. Astrophys., 463, 275-288 (2007)
	The onset of X-ray emission in young stellar objects. A Chandra observation of the Serpens star-forming region.
o	Table 5: <[GFM2007] NN> (Nos 1-85).
=E=	Catalogue in electronic form as J/A+A/463/275
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFR99]
[GFR99]	(Gurtler+Friedemann+Reimann+, 1999)
Write:	<<[GFR99] AA CCC a>>
N:	20+17+22+16
Object:	* (SIMBAD class: Star)
Note:	Comparison stars in the fields of 4 V*. In the case of SV Cep: updated version of the earlier identification map in 1992A&A...255..246F [FRG92]. Coordinates and missing letters added in 2000ARep...44..365R.
Ref:	=1999A&AS..140..293G
by	GUERTLER J. , FRIEDEMANN C., REIMANN H.-G., SPLITTGERBER E., RUDOLPH E.
	Astron. Astrophys., Suppl. Ser., 140, 293-307 (1999)
	A comparative study of the long-term light variations of six young irregular variables.
o	Table 2: <[GFR99] VX Cas a> (Nos a-v), <[GFR99] BH Cep a> (Nos a-s), <[GFR99] BO Cep a> (Nos a-x), <[GFR99] SV Cep a> (Nos a-t).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFS2003]
[GFS2003]	(Gaensler+Fogel+Slane+, 2003) (Not yet in Simbad)
Write:	<<[GFS2003] A>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of Tornado Nebula. N=3 extended regions of X-ray emission, (Nos A-C).
in source:	NAME Tornado Nebula
Ref:	=2003ApJ...594L..35G
by	GAENSLER B.M. , FOGEL J.K.J., SLANE P.O., MILLER J.M., WIJNANDS R., EIKENBERRY S.S., LEWIN W.H.G.
	Astrophys. J., 594, 35-38 (2003)
	Untwisting the Tornado: X-ray imaging and spectroscopy of G357.7-0.1.
o	Fig.1: <[GFS2003] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFS2006]
[GFS2006]	(Gonzalez-Martin+Fabian+Sanders, 2006)
Write:	<<[GFS2006] N>>
N:	8
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of NGC 1275.
in source:	NGC 1275 = 3C 84
Ref:	=2006MNRAS.367.1132G
by	GONZALEZ-MARTIN O. , FABIAN A.C., SANDERS J.S.
	Mon. Not. R. Astron. Soc., 367, 1132-1138 (2006)
	The ultraluminous X-ray sources in the high-velocity system of NGC1275.
o	in Chap. 4 : M51 X-1 is a misprint for M51 X-7.
o	Table 2: <[GFS2006] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFS2012]
[GFS2012]	(Getman+Feigelson+Sicilia-Aguilar+, 2012)
Write:	<<[GFS2012] NNN>> <<[GFS2012] IR NN>> <<[GFS2012] GN>> <<[GFS2012] G1267>>
N:	415+42+7+1
Object:	(X) + (MIR) + Stellar Group (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Chandra ACIS, FLWO and Calar Alto observations of IC 1396A. Use of Spitzer IRAC archival data. See also CXOIC1396A.
in source:	IC 1396A
Ref:	=2012MNRAS.426.2917G
by	GETMAN K.V. , FEIGELSON E.D., SICILIA-AGUILAR A., BROOS P.S., KUHN M.A., GARMIRE G.P.
	Mon. Not. R. Astron. Soc., 426, 2917-2943 (2012)
	The Elephant Trunk Nebula and the Trumpler 37 cluster: contribution of triggered star formation to the total population of an HII region.
o	Tables 1-3: <[GFS2012] NNN> (Nos 1-415) = Table 1, col(2): <CXOIC1396A JHHMMSS.ss+DDMMSS.s> N=415. Table 4: <[GFS2012] IR NN> (Nos 1-42). Fig. 13: <[GFS2012] GN> (Nos G1-G7), <[GFS2012] G1267> N=1.
=E=	Catalogue in electronic form as <J/MNRAS/426/2917/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFT2002]
[GFT2002]	(Getman+Feigelson+Townsley+, 2002)
Write:	<<[GFT2002] NNN>>
N:	109
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	The Chandra observations of NGC 1333 emitting young stars. See also CXONGC1333
in source:	NGC 1333
Ref:	=2002ApJ...575..354G
by	GETMAN K.V. , FEIGELSON E.D., TOWNSLEY L., BALLY J., LADA C.J., REIPURTH B.
	Astrophys. J., 575, 354-377 (2002)
	Chandra study of young stellar objects in the NGC 1333 star-forming cloud.
o	Table 1, col(1): <[GFT2002] NNN> (Nos 1-109) = Table 1, col(2): <CXONGC1333 JHHMMSS.s+DDMMSS> N=109.
=E=	Catalogue in electronic form as J/ApJ/575/354
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFT2006]
[GFT2006]	(Getman+Feigelson+Townsley+, 2006)
Write:	<<[GFT2006] NNN>>
N:	431
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra study of the Cep B molecular cloud. See also CXOCepB.
Ref:	=2006ApJS..163..306G
by	GETMAN K.V. , FEIGELSON E.D., TOWNSLEY L., BROOS P., GARMIRE G., TSUJIMOTO M.
	Astrophys. J., Suppl. Ser., 163, 306-334 (2006)
	Chandra study of the Cepheus B star-forming region: stellar populations and the initial mass function.
o	Table 1, col(1): <[GFT2006] NNN> (Nos 1-431) = Table 1, col(2): <CXOCepB JHHMMSS.ss+DDMMSS.s> N=431.
=E=	Catalogue in electronic form as J/ApJS/163/306
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFT2019]
[GFT2019]	(Gozaliasl+Finoguenov+Tanaka+, 2019)
Write:	<<[GFT2019] Group NNNNN>>
N:	247
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	N=247 X-ray groups of galaxies in the COSMOS field. Use of XMM-Newton and Chandra data. See also [FGH2007] and [GLB2011].
in source:	NAME COSMOS Field
Ref:	=2019MNRAS.483.3545G
by	GOZALIASL G. , FINOGUENOV A., TANAKA M., DOLAG K., MONTANARI F., KIRKPATRICK C.C., VARDOULAKI E., KHOSROSHAHI H.G., SALVATO M., LAIGLE C., McCRACKEN H.J., ILBERT O., CAPPELLUTI N., DADDI E., HASINGER G., CAPAK P., SCOVILLE N.Z., TOFT S., CIVANO F., GRIFFITHS R.E., BALOGH M., LI Y., AHORANTA J., MEI S., IOVINO A., HENRIQUES B.M.B., ERFANIANFAR G.
	Mon. Not. R. Astron. Soc., 483, 3545-3565 (2019)
	Chandra centres for COSMOS X-ray galaxy groups: differences in stellar properties between central dominant and offset brightest group galaxies.
o	Table 2: <[GFT2019] Group NNNNN> N=247 among (Nos 10006-30345).
=E=	Catalogue in electronic form as <J/MNRAS/483/3545/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFV2020]
[GFV2020]	(Gerber+Friel+Vesperini, 2020)
Write:	<<[GFV2020] NNNN>>
N:	151
Object:	* (SIMBAD class: Star)
Note:	WIYN Hydra spectroscopy of N=151 stars around the center of M71, selected using photometry from Cudworth (1985AJ.....90...65C and private communication). See also Cl* NGC 6838 KC.
in source:	NGC 6838 = M 71
Ref:	=2020AJ....159...50G
by	GERBER J.M. , FRIEL E.D., VESPERINI E.
	Astron. J., 159, 50-50 (2020)
	Identifying multiple populations in M71 using CN.
o	Table 1: <[GFV2020] NNNN> N=151 among (Nos 2-2299).
=E=	Catalogue in electronic form as <J/AJ/159/50/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GFW99]
[GFW99]	(Giannakopoulou-Creighton+Fich+Wilson, 1999)
Write:	<<[GFW99] NN>>
N:	10
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	N=10 Molecular Clouds in NGC 5461
in source:	NGC 5461
Ref:	=1999ApJ...522..238G
by	GIANNAKOPOULOU-CREIGHTON J. , FICH M., WILSON C.D.
	Astrophys. J., 522, 238-249 (1999)
	Star formation in the giant H II regions of M101.
o	Table 4: <[GFW99] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GG2000]
[GG2000]	(Grogin+Geller, 2000)
Write:	<<[GG2000] HHMMSS.ss+DDMMSS.s>>
N:	211
Object:	G (SIMBAD class: Galaxy)
Note:	See also Paper I: 1999AJ....118.2561G. [GG99].
Ref:	=2000AJ....119...32G
by	GROGIN N.A. , GELLER M.J.
	Astron. J., 119, 32-43 (2000)
	An imaging and spectroscopic survey of galaxies within prominent nearby voids. II. Morphologies, star formation, and faint companions.
o	Table 2: <[GG2000] HHMMSS.ss+DDMMSS.s> N=211.
=E=	Catalogue in electronic form as J/AJ/119/32
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GG2001]
[GG2001]	(Gabuzda+Gomez, 2001) (Not yet in Simbad)
Write:	<<[GG2001] OJ287 JN>> <<[GG2001] OJ287 A>>
N:	8+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	N=8 components in the jet of Ohio J 287, (Nos J1-J8), and N=1 Core 'C'.
in source:	OHIO J 287
Ref:	=2001MNRAS.320L..49G
by	GABUZDA D.C. , GOMEZ J.L.
	Mon. Not. R. Astron. Soc., 320, 49-54 (2001)
	VSOP polarization observations of the BL Lacertae object OJ 287.
o	Table 1: <[GG2001] OJ287 JN> (Nos J1-J8), <[GG2001] OJ287 A> (No. C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GG2005]
[GG2005]	(Georgantopoulos+Georgakakis, 2005)= (XBONG)
Write:	<<[GG2005] NN>>
N:	12
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Properties of X-ray Bright Optically inactive Galaxies (XBONGs) detected in XMM-Newton fields overlapping with the SDSS.
Ref:	=2005MNRAS.358..131G
by	GEORGANTOPOULOS I. , GEORGAKAKIS A.
	Mon. Not. R. Astron. Soc., 358, 131-138 (2005)
	X-ray bright optically inactive galaxies in XMM-Newton/Sloan Digital Sky Survey fields: more diluted than absorbed?
o	Table 1 : HAWAII 167 = [SCH94] 167.
o	Table 2: <[GG2005] NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GG2014]
[GG2014]	(Grenman+Gahm, 2014)
Write:	<<[GG2014] NNN>>
N:	288
Object:	Globulette (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	N=288 globulettes in the Carina complex. Use of archival HST Halpha images.
in source:	NAME CARINA REGION
Ref:	=2014A&A...565A.107G
by	GRENMAN T. , GAHM G.F.
	Astron. Astrophys., 565A, 107-107 (2014)
	The tiny globulettes in the Carina nebula.
o	Table A.1: <[GG2014] NNN> (Nos 1-288).
=E=	Catalogue in electronic form as J/A+A/565/A107
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GG2021]
[GG2021]	(Galiullin+Gilfanov, 2021)
Write:	<<[GG2021] NN>>
N:	39
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	N=39 super-soft X-ray sources (SSS) in eight nearby galaxies. Use of archival Chandra data.
Ref:	=2021A&A...646A..85G
by	GALIULLIN I. , GILFANOV M.
	Astron. Astrophys., 646A, 85-85 (2021)
	Populations of super-soft X-ray sources in galaxies of different morphological types.
o	Table C.1: <[GG2021] NN> (Nos 1-39).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GG52]
[GG52]	(Gonzalez+Gonzalez, 1952)= (G-G)
Write:	<<[GG52] NN>>
N:	71
Object:	* (SIMBAD class: Star)
Ref:	=1952BOTT....1e...8G
by	GONZALEZ G. , GONZALEZ G.
	Bol. Obs. Tonantz. Tacub., 1, part no 5, 8-None (1952)
	Estrellas de alta luminosidad en las vecindades de las constelaciones del Cisne y Cefeo.
o	<[GG52] NN> N=71
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GG53]
[GG53]	(Gonzalez+Gonzalez, 1953)= (G-G)
Write:	<<[GG53] NN>>
N:	29
Object:	* (SIMBAD class: Star)
Ref:	=1953BOTT....1g...3G
by	GONZALEZ G. , GONZALEZ G.
	Bol. Obs. Tonantz. Tacub., 1, part no 7, 3-10 (1953)
	Lista de estrellas de alta luminosidad.
o	<[GG53] NN> N=29
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GG70]
[GG70]	(Georgelin+Georgelin, 1970)= (An)
Write:	<<[GG70] An N>> <<[GG70] LLL.l+B.b>>
N:	8+4
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	N=8 HII regions, named 'An' (Anonym) by the authors. N=4 radio-sources.
Ref:	=1970A&A.....7..133G
by	GEORGELIN Y.P. , GEORGELIN Y.M.
	Astron. Astrophys., 7, 133-140 (1970)
	Prolongation du bras Sagittaire-Carene grace a trois regions HII lointaines.
o	T.1, text: <[GG70] An N> (Nos 1-8), <[GG70] LLL.l+B.b> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GG75]
[GG75]	(Geyer+Gieseking, 1975)
Write:	<<[GG75] NN>>
N:	28
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	Identif. charts
Ref:	=1975IBVS..967....1G
by	GEYER E.H. , GIESEKING F.
	IAU Inform. Bull. Var. Stars, 967, 1-2 (1975)
	Nine new variable stars in a field around µ Cep.
o	<[GG75] N> (Nos 1-9)
Ref:	=1976IBVS.1145....1G
by	GIESEKING F.
	IAU Inform. Bull. Var. Stars, 1145, 1-4 (1976)
	New variable Stars in the region of IC 1396.
o	<[GG75] NN> (Nos 10-28) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GG76]
[GG76]	(Georgelin+Georgelin, 1976)= (G	G)
Write:	<<[GG76] Group N>> <<[GG76] HII NNN>>
N:	9+100
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Table 7: N=9 HII groups (region complexes). Table 9: N=100 HII complexes.
Ref:	=1976A&A....49...57G
by	GEORGELIN Y.M. , GEORGELIN Y.P.
	Astron. Astrophys., 49, 57-79 (1976)
	The spiral structure of our galaxy determined from H II regions.
o	Table 7: <[GG76] Group N> (Nos 1-9). Table 9: <[GG76] HII NNN> (Nos 1-100)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GG99]
[GG99]	(Grogin+Geller, 1999)= (Century) = (15R)
Write:	<<[GG99] 15R FFF.NNNNNN>> <<[GG99] Century aNNNN.AA>>
N:	49+9
Object:	G (SIMBAD class: Galaxy)
Note:	End of table 2: N=49 galaxies from the 15R survey, here with a format 'FFF.NNNNNN', and N=9 galaxies from the Century survey, here with a format 'aNNNN.AA'
Ref:	=1999AJ....118.2561G
by	GROGIN N.A. , GELLER M.J.
	Astron. J., 118, 2561-2580 (1999)
	An imaging and spectroscopic survey of galaxies within prominent nearby voids. I. The sample and luminosity distribution.
o	Table 2: Galaxies format 'HHMMm+DDMM' are 'Z HHMM.m+DDMM'.
o	End of Table 2: <[GG99] Century aNNNN.AA> N=9, <[GG99] 15R FFF.NNNNNN> N=49.
=E=	Catalogue in electronic form as J/AJ/119/32
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GGA
GGA	(Gonzalez+Gonzalez, Anticenter)= (1G) = (G-G)
Write:	<<*Em GGA** NNN>>
N:	411
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Ref:	=1954BOTT....1i...3G
by	GONZALEZ G. , GONZALEZ G.
	Bol. Obs. Tonantz. Tacub., 1, part no 9, 3-20 (1954)
	Estrellas Be-Ae en Cassiopea y Perseo (Be and Ae stars).
o	<Em* GGA NNN> (Nos 1-192)
Ref:	=1956BOTT....2n..19G
by	GONZALEZ G. , GONZALEZ G.
	Bol. Obs. Tonantz. Tacub., 2, part no 14, 19-30 (1956)
	Estrellas con Hα en emission en longitudes galacticas de 103 a 180.
o	Table I: <Em* GGA NNN> (Nos 193-411)
Details on Acronym: [GGA2004]
[GGA2004]	(Georgantopoulos+Georgakakis+Akylas+, 2004)
Write:	<<[GGA2004] NN>>
N:	61
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	N=61 hard X-ray sources from the bright XMM-Newton/2dF survey. See also paper I: XMM2DF.
Ref:	=2004MNRAS.352...91G
by	GEORGANTOPOULOS I. , GEORGAKAKIS A., AKYLAS A., STEWART G.C., GIANNAKIS O., SHANKS T., KITSIONAS S.
	Mon. Not. R. Astron. Soc., 352, 91-100 (2004)
	The XMM-Newton/2dF survey - IV. The X-ray spectral properties of the hard sources.
o	Table 2: <[GGA2004] NN> (Nos 1-61).
=E=	Catalogue in electronic form as J/MNRAS/352/91
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGA2006]
[GGA2006]	(Georgakakis+Georgantopoulos+Akylas, 2006)
Write:	<<[GGA2006] NN>>
N:	84
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton archival observations selected to overlap with the DR2 SDSS to explore the nature of the X-ray sources with red optical colours. 84 AGN candidates are found.
Ref:	=2006MNRAS.366..171G
by	GEORGAKAKIS A.E. , GEORGANTOPOULOS I., AKYLAS A.
	Mon. Not. R. Astron. Soc., 366, 171-181 (2006)
	Red active galactic nuclei in XMM-Newton/Sloan Digital Sky Survey fields.
o	Table 1: <[GGA2006] NN> (Nos 1-84).
=E=	Catalogue in electronic form as J/MNRAS/366/171
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGA2007]
[GGA2007]	(Gilmour+Gray+Almaini+, 2007)
Write:	<<[GGA2007] NNN>>
N:	139
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton data for the supercluster ACO901-902.
in source:	NAME ACO 901-902 Supercluster
Ref:	=2007MNRAS.380.1467G
by	GILMOUR R. , GRAY M.E., ALMAINI O., BEST P., WOLF C., MEISENHEIMER K., PAPOVICH C., BELL E.
	Mon. Not. R. Astron. Soc., 380, 1467-1487 (2007)
	Environmental dependence of active galactic nuclei activity in the supercluster A901/2.
o	Table 1: <[GGA2007] NNN> (Nos 1-139).
=E=	Catalogue in electronic form as J/MNRAS/380/1467
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGA99]
[GGA99]	(Glass+Ganesh+Alard+, 1999)= (BW)
Write:	<<[GGA99] NGC 6522 NNN>> <<[GGA99] Sgr I NNN>>
N:	142+216
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Bright sources from the ISOGAL project, in NGC 6522 field (MACHO field 119), or in Sgr I field (MACHO field 113). See also ISOGAL-P.
Ref:	=1999MNRAS.308..127G
by	GLASS I.S. , GANESH S., ALARD C., BLOMMAERT J.A.D.L., GILMORE G., LLOYD EVANS T., OMONT A., SCHULTHEIS M., SIMON G.
	Mon. Not. R. Astron. Soc., 308, 127-139 (1999)
	ISOGAL survey of Baade's Windows in the mid-infrared.
o	Notes to Tables 2 and 3: B = stars classified by Blanco, 1986 (not BMB).
o	Table 2: <[GGA99] NGC 6522 NNN> N=33 among 497 = <ISOGAL-P JHHMMSS.s+DDMMSS> N=33. Table 3: <[GGA99] Sgr I NNN> N=64 among 696 = <ISOGAL-P JHHMMSS.s+DDMMSS> N=64.
Ref:	=2001ApJ...552..289A
by	ALARD C. , BLOMMAERT J.A.D.L., CESARSKY C., EPCHTEIN N., FELLI M., FOUQUE P., GANESH S., GENZEL R., GILMORE G., GLASS I.S., HABING H., OMONT A., PERAULT M., PRICE S., ROBIN A., SCHULTHEIS M., SIMON G., VAN LOON J.T., ALCOCK C., ALLSMAN R.A., ALVES D.R., AXELROD T.S., BECKER A.C., BENNETT D.P., COOK K.H., DRAKE A.J., FREEMAN K.C., GEHA M., GRIEST K., LEHNER M.J., MARSHALL S.L., MINNITI D., NELSON C., PETERSON B.A., POPOWSKI P., PRATT M.R., QUINN P.J., SUTHERLAND W., TOMANEY A.B., VANDEHEI T., WELCH D.L.
	Astrophys. J., 552, 289-308 (2001)
	Mass-losing semiregular variable stars in Baade's windows.
o	Table 1: <ISOGAL-P JHHMMSS.s+DDMMSS> N=332 = <[GGA99] NGC 6522 NNN> N=109 new, or = [GGA99] Sgr I NNN> N=152 new.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGB2004]
[GGB2004]	(Georgakakis+Georgantopoulos+Basilakos+, 2004)
Write:	<<[GGB2004] NN>>
N:	17
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	First results from a survey aiming at identifying X-ray selected normal galaxies by combining archival XMM-Newton data with the SDSS.
Ref:	=2004MNRAS.354..123G
by	GEORGAKAKIS A.E. , GEORGANTOPOULOS I., BASILAKOS S., PLIONIS M., KOLOKOTRONIS V.
	Mon. Not. R. Astron. Soc., 354, 123-126 (2004)
	The Needles in the Haystack Survey: searching for X-ray-selected normal galaxies.
o	Table 1: <[GGB2004] NN> (Nos 1-17).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGB2010]
[GGB2010]	(Guzman+Garay+Brooks, 2010)
Write:	<<[GGB2010] C>> <<[GGB2010] A-W>>
N:	1+4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA 1.4, 2.4, 4.8, and 8.6cm observations of N=5 radio components detected toward IRAS 16562-3959.
Ref:	=2010ApJ...725..734G
by	GUZMAN A.E. , GARAY G., BROOKS K.J.
	Astrophys. J., 725, 734-741 (2010)
	A string of radio emission associated with IRAS 16562-3959: a collimated jet emanating from a luminous massive young stellar object.
o	Fig. 1 ,Table 1: <[GGB2010] C> N=1, <[GGB2010] W-W> (Nos I-E, I-W, O-E, O-W).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGB2012]
[GGB2012]	(Guzman+Garay+Brooks+, 2012)
Write:	<<[GGB2012] GLLL.llll+BB.bbbb A>>
N:	33 (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Ref:	=2012ApJ...753...51G
by	GUZMAN A.E. , GARAY G., BROOKS K.J., VORONKOV M.A.
	Astrophys. J., 753, 51 (2012)
	Search for ionized jets toward high-mass young stellar objects.
o	(Erratum) erratum vol. 781, art. 56 (2014)
o	<[GGB2012] GLLL.llll+BB.bbbb A> N=33.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGB2019]
[GGB2019]	(Gonzalez+Gettings+Brodwin+, 2019)
Write:	<<[GGB2019] JHHMMSS.ss+DDMMSS.s>>
N:	7
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	GTC OSIRIS spectroscopic observations of N=7 galaxies, members of the cluster MOO J1229+6521. See also [GGS2012] and [GDB2015].
in source:	PSZ2 G126.57+51.61 = MOO J1229+6521
Ref:	=2019ApJS..240...33G
by	GONZALEZ A.H. , GETTINGS D.P., BRODWIN M., EISENHARDT P.R.M., STANFORD S.A., WYLEZALEK D., DECKER B., MARRONE D.P., MORAVEC E., O'DONNELL C., STALDER B., STERN D., ABDULLA Z., BROWN G., CARLSTROM J., CHAMBERS K.C., HAYDEN B., LIN Y.-T., MAGNIER E., MASCI F.J., MANTZ A.B., McDONALD M., MO W., PERLMUTTER S., WRIGHT E.L., ZEIMANN G.R.
	Astrophys. J., Suppl. Ser., 240, 33-33 (2019)
	The Massive and Distant Clusters of WISE Survey. I. Survey overview and a catalog of >2000 galaxy clusters at z ≃ 1.
o	Tables 3-5: <MOO JHHMM+DDMM> N=2433+250+156. Table 7: <[GGB2019] JHHMMSS.ss+DDMMSS.s> N=7.
=E=	Catalogue in electronic form as <J/ApJS/240/33/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGC2003]
[GGC2003]	(Guainazzi+Grandi+Comastri+, 2003)
Write:	<<[GGC2003] N>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	BeppoSAX observations of the field around NGC 6251. Use of archival ASCA and Chandra data. The three sources are detected in Chandra ACIS-I data.
Ref:	=2003A&A...410..131G
by	GUAINAZZI M. , GRANDI P., COMASTRI A., MATT G.
	Astron. Astrophys., 410, 131-138 (2003)
	The hard X-ray view of the low-luminosity blazar in the radio galaxy NGC 6251.
o	In reflist, Sudou PASJ.52 : read 2000 instead of 2001.
o	Table 4: <[GGC2003] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGC2005]
[GGC2005]	(Guziy+Gorosabel+Castro-Tirado+, 2005)
Write:	<<[GGC2005] A>> <<[GGC2005] N>>
N:	3+4
Object:	* + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	ESO 3.6m telescope at La Silla observations of the field of GRB 000214: 3 standard stars are used, and 4 possible host galaxies of the GRB are found.
Ref:	=2005A&A...441..975G
by	GUZIY S. , GOROSABEL J., CASTRO-TIRADO A.J., DE UGARTE POSTIGO A., JELINEK M., PEREZ RAMIREZ M.D., CASTRO CERON J.M., KLOSE S., PALAZZI E., WIERSEMA K.
	Astron. Astrophys., 441, 975-979 (2005)
	The search for the host galaxy of the γ-ray burst GRB 000214.
o	Table 2: <[GGC2005] A> (Nos A-C). Table 3: <[GGC2005] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGC2008]
[GGC2008]	(Grossi+Giovanardi+Corbelli+, 2008)
Write:	<<[GGC2008] AANNa>>
N:	24
Object:	HI Cloud (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	Arecibo Legacy Fast ALFA (AA in the format) survey. Search for neutral hydrogen clouds in the field of M 33.
Ref:	=2008A&A...487..161G
by	GROSSI M. , GIOVANARDI C., CORBELLI E., GIOVANELLI R., HAYNES M.P., MARTIN A.M., SAINTONGE A., DOWELL J.D.
	Astron. Astrophys., 487, 161-175 (2008)
	HI clouds in the proximity of M 33.
o	Tables 1, 2: <[GGC2008] AANNa> (Nos 1-20, 21a-21b, 22-23).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGC2012]
[GGC2012]	(Gullieuszik+Groenewegen+Cioni+, 2012)
Write:	<<[GGC2012] JHHMMSS.ss+DDMMSS.s>>
N:	374
Object:	Poss. AGB (SIMBAD class: AGB*_Candidate = Asymptotic Giant Branch Star Candidate)
Note:	N=374 AGB candidates in one of the fields observed by the VISTA survey of the Magellanic Clouds (VMC).
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2012A&A...537A.105G
by	GULLIEUSZIK M. , GROENEWEGEN M.A.T., CIONI M.-R.L., DE GRIJS R., VAN LOON J.T., GIRARDI L., IVANOV V.D., OLIVEIRA J.M., EMERSON J.P., GUANDALINI R.
	Astron. Astrophys., 537A, 105-105 (2012)
	The VMC survey. III. Mass-loss rates and luminosities of LMC AGB stars.
o	Tables 2+6: <[GGC2012] JHHMMSS.ss+DDMMSS.s> N=374.
=E=	Catalogue in electronic form as J/A+A/537/A105
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGC82]
[GGC82]	(Gehrz+Grasdalen+Castelaz+, 1982)= (IRS)
Write:	<<[GGC82] IRS NW>> <<[GGC82] a>>
N:	9+4+3
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	N=9 Infrared sources in Sh 2-106, 'IRS N' (Nos 1-8), source 3 having 4 components (3N, 3S and 3E, 3W). N=3 compact sources (Nos a-c).
in source:	SH 2-106
Ref:	=1982ApJ...254..550G
by	GEHRZ R.D. , GRASDALEN G.L., CASTELAZ M., GULLIXSON C., MOZURKEWICH D., HACKWELL J.A.
	Astrophys. J., 254, 550-561 (1982)
	Anatomy of a region of star formation: infrared images of S 106 (AFGL 2584).
o	Table 1: <[GGC82] IRS N> (Nos 1-8). Table 2: <[GGC82] a> (Nos a-c)
Ref:	=1982A&A...116..179H
by	HOFMANN R.G.
	Astron. Astrophys., 116, 179-182 (1982)
	A new near-infrared source in the molecular cloud associated with S 106.
o	<[GGC82] IRS N> (No. 9) added.
Ref:	=1988ApJ...326..339P
by	PERSSON S.E. , McGREGOR P.J., CAMPBELL B.
	Astrophys. J., 326, 339-355 (1988)
	High spatial and spectral resolution observations of the optical counterparts of GL 490 and S 106/IRS 3.
o	Table 1: <[GGC82] IRS 3W> (Nos 3W, 3E, 3S).
Ref:	=1990MNRAS.246..565A
by	ASPIN C. , RAYNER J.T., McLEAN I.S., HAYASHI S.S.
	Mon. Not. R. Astron. Soc., 246, 565-575 (1990)
	Infrared polarimetry and photometry of S 106.
o	Table 1: <[GGC82] IRS 3W> (No. 3N) added. Tables 1, 2, Fig.2: <[ARM90] R> (Nos I to VII).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GGD
GGD	(Gyulbudaghian+Glushkov+Denisyuk)
Write:	<<GGD NN>> <<GGD NNa>>
N:	37
Object:	Poss. HH (SIMBAD class: HerbigHaroObj = Herbig-Haro Object)
Note:	(Nos 1-36) are identical to GM 2-NN (Nos 1-36) See GM.
Ref:	=1978ApJ...224L.137G
by	GYULBUDAGHIAN A.L. , GLUSHKOV Y.I., DENISYUK E.K.
	Astrophys. J., 224, 137-138 (1978)
	New Herbig-Haro objects.
o	<GGD NN> (Nos 1-37)
Details on Acronym: GGE
GGE	(Gonzalez+Gonzalez, Early type)= (2G) = (G-G) (Not yet in Simbad)
Write:	<<GGE NNN>>
N:	150
Object:	OB* (SIMBAD class: Star)
Ref:	=1954BOTT....2k..25G
by	GONZALEZ G. , GONZALEZ G.
	Bol. Obs. Tonantz. Tacub., 2, part no 11, 25-26 (1954)
	Gigantes azules en las longitudes galacticas 270 D a 330 D.
o	Table 1: <GGE NNN> (Nos 1-150).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGF2007]
[GGF2007]	(Gahm+Grenman+Fredriksson+, 2007)= (Globulette)
Write:	<<[GGF2007] NGC 7822 N>> <<[GGF2007] IC 1805 NN>> <<[GGF2007] Rosette Nebula NNN>> <<[GGF2007] NGC 6820 N>>
N:	9+18+145+1
Object:	Globulette (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	H-alpha images of HII regions collected with the 2.6m Optical Telescope on La Palma. Tiny dusty clouds, much smaller than normal globules, are designated as globulettes by the authors.
in source:	NGC 7822
in source:	IC 1805
in source:	NAME Rosette Nebula
in source:	NGC 6820
Ref:	=2007AJ....133.1795G
by	GAHM G.F. , GRENMAN T., FREDRIKSSON S., KRISTEN H.
	Astron. J., 133, 1795-1809 (2007)
	Globulettes as seeds of brown dwarfs and free-floating planetary-mass objects.
o	Table 2: <[GGF2007] NGC 7822 N> (Nos 1-9), <[GGF2007] IC 1805 NN> (Nos 1-18), <[GGF2007] Rosette Nebula NNN> (Nos 1-145), <[GGF2007] NGC 6820 N> (No. 1).
=E=	Catalogue in electronic form as J/AJ/133/1795
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGF2011]
[GGF2011]	(Gusdorf+Giannini+Flower+, 2011)
Write:	<<[GGF2011] SiO peak>> <<[GGF2011] SiO knot>>
N:	1+1
Object:	Outflow (SIMBAD class: Outflow)
Stat:	is completely incorporated in Simbad
Note:	APEX SiO observations of a bipolar outflow region in the Bok globule BHR 71.
in source:	BHR 71
Ref:	=2011A&A...532A..53G
by	GUSDORF A. , GIANNINI T., FLOWER D.R., PARISE B., GUESTEN R., KRISTENSEN L.E.
	Astron. Astrophys., 532A, 53-53 (2011)
	Revisiting the shocks in BHR 71: new observational constraints and H_{2}O predictions for Herschel.
o	Fig. 1, Table 1: <[GGF2011] SiO peak> N=1, <[GGF2011] SiO knot> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGF2012]
[GGF2012]	(Guo+Giavalisco+Ferguson+, 2012)
Write:	<<[GGF2012] NNNNN>> <<[GGF2012] NNNNN N>>
N:	10+41
Object:	G + Part of G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST ACS and WFC3 observations of the Hubble Ultra Deep Field.
in source:	NAME Hubble Ultra Deep Field
Ref:	=2012ApJ...757..120G
by	GUO Y. , GIAVALISCO M., FERGUSON H.C., CASSATA P., KOEKEMOER A.M.
	Astrophys. J., 757, 120 (2012)
	Multi-wavelength view of kiloparsec-scale clumps in star-forming galaxies at z ~ 2.
o	Table 1: <[GGF2012] NNNNN> N=10 among (Nos 20565-27101). Table 2: <[GGF2012] NNNNN N> N=41.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGF2013]
[GGF2013]	(Galametz+Grazian+Fontana+, 2013)
Write:	<<[GGF2013] NNNNN>>
N:	35932
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Catalog of N=35932 F160W-selected sources in the UKIDSS UDS field, as part of the CANDELS survey. See also CANDELS UDS F160W.
Ref:	=2013ApJS..206...10G
by	GALAMETZ A. , GRAZIAN A., FONTANA A., FERGUSON H.C., ASHBY M.L.N., BARRO G., CASTELLANO M., DAHLEN T., DONLEY J.L., FABER S.M., GROGIN N., GUO Y., HUANG K.-H., KOCEVSKI D.D., KOEKEMOER A.M., LEE K.-S., McGRATH E.J., PETH M., WILLNER S.P., ALMAINI O., COOPER M., COORAY A., CONSELICE C.J., DICKINSON M., DUNLOP J.S., FAZIO G.G., FOUCAUD S., GARDNER J.P., GIAVALISCO M., HATHI N.P., HARTLEY W.G., KOO D.C., LAI K., DE MELLO D.F., McLURE R.J., LUCAS R.A., PARIS D., PENTERICCI L., SANTINI P., SIMPSON C., SOMMARIVA V., TARGETT T., WEINER B.J., WUYTS S., (The CANDELS Team)
	Astrophys. J., Suppl. Ser., 206, 10 (2013)
	CANDELS multiwavelength catalogs: source identification and photometry in the CANDELS UKIDSS ultra-deep survey field.
o	Table 3: <[GGF2013] NNNNN> (Nos 1-35932) = <CANDELS UDS F160W JHHMMSS.ss+DDMMSS.s> N=35932.
=E=	Catalogue in electronic form as J/ApJS/206/10
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGG2013]
[GGG2013]	(Gitti+Giroletti+Giovannini+, 2013)
Write:	<<[GGG2013] CN>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	EVN 5GHz observations of N=2 compact components in the brightest cluster galaxy of RBS 797.
in source:	NAME RBS 797 BCG
Ref:	=2013A&A...557L..14G
by	GITTI M. , GIROLETTI M., GIOVANNINI G., FERETTI L., LIUZZO E.
	Astron. Astrophys., 557L, 14-14 (2013)
	A candidate supermassive binary black hole system in the brightest cluster galaxy of RBS 797.
o	Fig. 1: <[GGG2013] CN> (Nos C1-C2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGG2016]
[GGG2016]	(Ginsburg+Goss+Goddi+, 2016)
Write:	<<[GGG2016] W51aNNw>> <<[GGG2016] W51aNNd>> <<[GGG2016] W51aNNmol>> <<[GGG2016] arc>>
N:	30+3+2+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	JVLA S and C band observations of the W51 protocluster complex.
in source:	W 51
Ref:	=2016A&A...595A..27G
by	GINSBURG A. , GOSS W.M., GODDI C., GALVAN-MADRID R., DALE J.E., BALLY J., BATTERSBY C.D., YOUNGBLOOD A., SANKRIT R., SMITH R., DARLING J., KRUIJSSEN J.M.D., LIU H.B.
	Astron. Astrophys., 595A, 27-27 (2016)
	Toward gas exhaustion in the W51 high-mass protoclusters.
o	Fig. 2, Table 3: <W 51aNN> (Nos W 51d3-d7, W 51e9-e23) added. Figs 2+A.2, Tables 3-8: <[GGG2016] arc> N=1, <[GGG2016] W51aNNw> (Nos W51d3, W51d4e-W51d4w, W51d5-W51d7, W51e8n-W51e8s, W51e9-23), <[GGG2016] W51aNNd> (Nos W51d3d, W51e11d, W51e18d), <[GGG2016] W51aNNmol> (Nos W51e8mol, W51e10mol).
=E=	Catalogue in electronic form as <J/A+A/595/A27/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGH2002]
[GGH2002]	(Groenewegen+Girardi+Hatziminaoglou+, 2002)= (EIS)
Write:	<<[GGH2002] EIS JHHMMSS.ss+DDMMSS.s>>
N:	1659
Object:	* + G + QSO (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	EIS catalogue in Chandra Deep Field South.
in source:	NAME CDFS
Ref:	=2002A&A...392..741G
by	GROENEWEGEN M.A.T. , GIRARDI L., HATZIMINAOGLOU E., BENOIST C., OLSEN L.F., DA COSTA L., ARNOUTS S., MADEJSKY R., MIGNANI R.P., RITE C., SIKKEMA G., SLIJKHUIS R., VANDAME B.
	Astron. Astrophys., 392, 741-755 (2002)
	ESO Imaging Survey. The stellar catalogue in the Chandra Deep Field South.
o	J033138.80-274460.0 is J033138.80-274500.0; J033240.53-274360.0 is J033240.53-274400.0
o	Tables 3-8: <[GGH2002] EIS JHHMMSS.ss+DDMMSS.s> N=1659.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGH2005]
[GGH2005]	(Giles+Greenhill+Hill+, 2005) (Not yet in Simbad)
Write:	<<[GGH2005] N>>
N:	5
Object:	* (SIMBAD class: Star)
Note:	Standard stars in the field of XTE J0929-314.
Ref:	=2005MNRAS.361.1180G
by	GILES A.B. , GREENHILL J.G., HILL K.M., SANDERS E.
	Mon. Not. R. Astron. Soc., 361, 1180-1186 (2005)
	The optical counterpart of XTE J0929-314: the third transient millisecond X-ray pulsar.
o	Table 1, Fig.1: <[GGH2005] N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGH2006]
[GGH2006]	(Gomez+Geisler+Harris+, 2006)
Write:	<<[GGH2006] NNN>>
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	Magellan I 6.5m telescope at Las Campanas Observatory images of NGC 5128. Search for new (N in the format) globular clusters. See also [WHH2005].
in source:	NGC 5128 = Cen A
Ref:	=2006A&A...447..877G
by	GOMEZ M. , GEISLER D., HARRIS W.E., RICHTLER T., HARRIS G.L.H., WOODLEY K.A.
	Astron. Astrophys., 447, 877-890 (2006)
	Structural parameters from ground-based observations of newly discovered globular clusters in NGC 5128.
o	Paragraph 5.1. objects WHH094, WHH127 and WHH43: WHH list ([WHH2005] in Simbad) has only 31 objects, WHH is here a misprint for HHG, these objects are [HHG2004] 94, [HHG2004] 127 and [HHG2004] 43 in Simbad.
o	Table 2: <[GGH2006] ANN> N=23 among (Nos N1-N42).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGH82]
[GGH82]	(Gioia+Geller+Huchra+, 1982)
Write:	<<[GGH82] AN>> <<[GGH82] NN>>
N:	5+12
Object:	(X) + (Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Einstein HRI X and MMT optical observations of the cluster Abell 2069.
in source:	ACO 2069
Ref:	=1982ApJ...255L..17G
by	GIOIA I.M. , GELLER M.J., HUCHRA J.P., MACCACARO T., STEINER J.E., STOCKE J.
	Astrophys. J., 255, 17-21 (1982)
	Abell 2069: an X-ray cluster of galaxies with multiple subcondensations.
o	Fig. 1, Table 1: <[GGH82] AN> (Nos A, A1-A3, B). Fig. 2, Table 2: <[GGH82] NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGK2003]
[GGK2003]	(Greiner+Guenther+Klose+, 2003)
Write:	<<[GGK2003] GRB 030226 abs N.NNN>>
N:	2
Object:	Absorber
Note:	VLT FORS2 spectrographic observations of GRB 030226. See also [PFD2003].
Ref:	=2003GCN..1886....1G
by	GREINER J. , GUENTHER E., KLOSE S., SCHWARZ R.
	GRB Coordinates Network, Circular Service, 1886, 1-None (2003)
	Two absorption systems in GRB 030226.
o	<[GGK2003] GRB 030226 abs N.NNN> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGK2005]
[GGK2005]	(Georgantopoulos+Georgakakis+Koulouridis, 2005)
Write:	<<[GGK2005] NN>>
N:	31
Object:	G (SIMBAD class: Galaxy)
Note:	XMM-Newton observations of X-ray selected normal galaxies.
Ref:	=2005MNRAS.360..782G
by	GEORGANTOPOULOS I. , GEORGAKAKIS A., KOULOURIDIS E.
	Mon. Not. R. Astron. Soc., 360, 782-790 (2005)
	The XMM-Newton Needles in the Haystack Survey: the local X-ray luminosity function of `normal' galaxies.
o	In table 1 : Hawaii 167 = [SCH94] 167.
o	Table 2: <[GGK2005] NN> (Nos 1-31).
=E=	Catalogue in electronic form as J/MNRAS/360/782
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGK2017]
[GGK2017]	(Ginsburg+Goddi+Kruijssen+, 2017)
Write:	<<[GGK2017] ALMAmmNN>> <<[GGK2017] aN>> <<[GGK2017] e2e>> <<[GGK2017] e2e peak>> <<[GGK2017] e2ww>> <<[GGK2017] eNmmN>> <<[GGK2017] eWmmNa>> <<[GGK2017] north>>
N:	57+2+1+1+3+3+9+1
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	ALMA 1.3mm observations of N=77 continuum sources in the high-mass protocluster W 51.
in source:	W 51
Ref:	=2017ApJ...842...92G
by	GINSBURG A. , GODDI C., KRUIJSSEN J.M.D., BALLY J., SMITH R., GALVAN-MADRID R., MILLS E.A.C., WANG K., DALE J.E., DARLING J., ROSOLOWSKY E., LOUGHNANE R., TESTI L., BASTIAN N.
	Astrophys. J., 842, 92-92 (2017)
	Thermal feedback in the high-mass star and cluster forming region W51.
o	Tables 7-8: <[GGK2017] ALMAmmNN> (Nos 1-57). Table 8: <[GGK2017] aN> (Nos d2, e5), <[GGK2017] e2e> N=1, <[GGK2017] e2e peak> N=1, <[GGK2017] e2ww> (Nos e2nw, e2se, e2w), <[GGK2017] eNmmN> (Nos e1mm1, e3mm1, e8mm), <[GGK2017] eWmmNa> (Nos eEmm1-eEmm3, eSmm1-eSmm2, eSmm2a, eSmm3-eSmm6), <[GGK2017] north> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGL95]
[GGL95]	(Gomez+Garay+Lizano, 1995)
Write:	<<[GGL95] G32.80 A>> <<[GGL95] G32.80 W>> <<[GGL95] G61.48 W>>
N:	3+2
Object:	Clump (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=3 Ammonia clumps in the HII region [WAM82] 032.797+0.192: North, Middle, AND South clumps, (Nos N, M, S). N=2 Ammonia clumps in the HII region [WC89] 061.48+0.09: East and West clumps, (Nos E, W).
in source:	[WAM82] 032.797+0.192
in source:	[WC89] 061.48+0.09
Ref:	=1995ApJ...453..727G
by	GOMEZ Y. , GARAY G., LIZANO S.
	Astrophys. J., 453, 727-740 (1995)
	Warm molecular gas associated with cometary H II regions.
o	Table 1: G32.80+0.19A and B = [GRM93] G32.80+0.19A and B, G61.48+0.09B1 and B2 = [L74] Sh 2-88 B1 and B2.
o	Table 2: <[GGL95] G32.80 W> (Nos N, M, S), <[GGL95] G61.48 W> (Nos E, W).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGM2003]
[GGM2003]	(Grandi+Guainazzi+Maraschi+, 2003)
Write:	<<[GGM2003] JHHMMSS.s+DDMMSS.s>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of Pictoris A: N=2 point-like foreground objects in the eastern lobe.
in source:	NAME Pic A
Ref:	=2003ApJ...586..123G
by	GRANDI P. , GUAINAZZI M., MARASCHI L., MORGANTI R., FUSCO-FEMIANO R., FIOCCHI M., BALLO L., TAVECCHIO F.
	Astrophys. J., 586, 123-127 (2003)
	Detection of X-ray emission from the eastern radio lobe of Pictor A.
o	Fig.1: <[GGM2003] JHHMMSS.s+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGM2006]
[GGM2006]	(Gettel+Geske+McKay, 2006)
Write:	<<[GGM2006] NNNNNNNN>>
N:	1022
Object:	(SIMBAD class: = Double or Multiple Star)
Stat:	is completely incorporated in Simbad
Note:	Sample of contact binary stars extracted from sky patrol data taken by the ROTSE-I telescope.
Ref:	=2006AJ....131..621G
by	GETTEL S.J. , GESKE M.T., McKAY T.A.
	Astron. J., 131, 621-632 (2006)
	A catalog of 1022 bright contact binary stars.
o	Catalog: <[GGM2006] NNNNNNNN> N=1022.
=E=	Catalogue in electronic form as J/AJ/131/621
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGM2011]
[GGM2011]	(Giraud+Gu+Melnick+, 2011)
Write:	<<[GGM2011] NNNNa>>
N:	676
Object:	G (SIMBAD class: Galaxy)
Note:	VLT FORS2 observations of a field centered on the X-ray cluster RX J0054.0-2823.
in source:	RX J0054.0-2823
Ref:	=2011RAA....11..245G
by	GIRAUD E. , GU Q.-S., MELNICK J., QUINTANA H., SELMAN F., TOLEDO I., ZELAYA P.
	RAA, 11, 245-270 (2011)
	Low-ionization galaxies and evolution in a pilot survey up to z = 1.
o	Table 5: <[GGM2011] NNNNa> N=676 among (Nos 1-1020).
=E=	Catalogue in electronic form as J/other/RAA/11.245
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGM2014]
[GGM2014]	(Green+Glazebrook+McGregor+, 2014)
Write:	<<[GGM2014] A NN-N>>
N:	67
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	AAT AAOmega/SPIRAL and ANU WiFeS integral-field spectroscopy of N=67 galaxies selected from the SDSS.
Ref:	=2014MNRAS.437.1070G
by	GREEN A.W. , GLAZEBROOK K., McGREGOR P.J., DAMJANOV I., WISNIOSKI E., ABRAHAM R.G., COLLESS M., SHARP R.G., CRAIN R.A., POOLE G.B., McCARTHY P.J.
	Mon. Not. R. Astron. Soc., 437, 1070-1095 (2014)
	DYNAMO - I. A sample of Hα-luminous galaxies with resolved kinematics.
o	Table 3: <[GGM2014] A NN-N> N=67.
=E=	Catalogue in electronic form as J/MNRAS/437/1070
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGM98]
[GGM98]	(Gaensler+Green+Manchester, 1998)= (ATCA)
Write:	<<[GGM98] ATCA JHHMMSS+DDMMSS>> <<[GGM98] Source N>> <<[GGM98] Region A>>
N:	1+3+4
Object:	? (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=1 radio-source 'ATCA J134649-625235' NE of the centre of SNR 309.2-00.6, and N=3 other sources (Nos 1-3) in the vicinity of the SNR. Fig.4: N=4 regions (Nos A-D) in the SNR.
in source:	SNR G309.2-00.6
Ref:	=1998MNRAS.299..812G
by	GAENSLER B.M. , GREEN A.J., MANCHESTER R.N.
	Mon. Not. R. Astron. Soc., 299, 812-824 (1998)
	G309.2-00.6 and jets in supernova remnants.
o	Table 2: <[GGM98] ATCA J134649-625235> N=1, <[GGM98] Source N> (Nos 1-3). Fig.4: <[GGM98] Region A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGP2003]
[GGP2003]	(Ganeshalingam+Graham+Pugh+, 2003)
Write:	<<[GGP2003] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of SN 2003EK.
Ref:	=2003IAUC.8134....1G
by	GANESHALINGAM M. , GRAHAM J., PUGH H., LI W.
	IAU Circ., 8134, 1-None (2003)
	Supernovae 2003ef, 2003eg, 2003eh, 2003ei, 2003ej, 2003ek.
o	<[GGP2003] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGP2008]
[GGP2008]	(Georgiev+Goudfrooij+Puzia+, 2008)
Write:	<<[GGP2008] EFFF-NNN-NN>> <<[GGP2008] NNNNN-NN>> <<[GGP2008] IC1959-NN>> <<[GGP2008] KKNN-NN>> <<[GGP2008] UNNNN-NN>>
N:	60
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	HST ACS images of 16 galaxies to search for old clusters. See also [GPH2009].
Ref:	=2008AJ....135.1858G
by	GEORGIEV I.Y. , GOUDFROOIJ P., PUZIA T.H., HILKER M.
	Astron. J., 135, 1858-1876 (2008)
	Old globular clusters in Magellanic-type dwarf irregular galaxies.
o	Table 3: <[GGP2008] EFFF-NNN-NN>, <[GGP2008] ANNNN-NN>, <[GGP2008] IC1959-NN>, <[GGP2008] KKNN-NN>, <[GGP2008] UNNNN-NN>, N=60.
=E=	Catalogue in electronic form as J/AJ/135/1858
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGP2014]
[GGP2014]	(Grillo+Gobat+Presotto+, 2014)
Write:	<<[GGP2014] MACS J1206.2-0847 GN>> <<[GGP2014] MACS J1206.2-0847 AN>>
N:	2+10
Object:	Grav. lensed image + Grav. lens (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	VLT VIMOS and FORS2 spectroscopic observations of two early-type galaxies in the field of the galaxy cluster MACS J1206.2-0847.
in source:	MCS J1206.2-0847
Ref:	=2014ApJ...786...11G
by	GRILLO C. , GOBAT R., PRESOTTO V., BALESTRA I., MERCURIO A., ROSATI P., NONINO M., VANZELLA E., CHRISTENSEN L., GRAVES G., BIVIANO A., LEMZE D., BARTELMANN M., BENITEZ N., BOUWENS R., BRADLEY L., BROADHURST T., COE D., DONAHUE M., FORD H., INFANTE L., JOUVEL S., KELSON D., KOEKEMOER A., LAHAV O., MEDEZINSKI E., MELCHIOR P., MENEGHETTI M., MERTEN J., MOLINO A., MONNA A., MOUSTAKAS J., MOUSTAKAS L.A., POSTMAN M., SEITZ S., UMETSU K., ZHENG W., ZITRIN A.
	Astrophys. J., 786, 11 (2014)
	CLASH: extending galaxy strong lensing to small physical scales with distant sources highly magnified by galaxy cluster members.
o	Table 1: <[GGP2014] MACS J1206.2-0847 GN> (Nos G1-G2). Table 2: <[GGP2014] MACS J1206.2-0847 AN> (Nos A1-B1, A2-B2, A3-B3, A4-B4, A5-B5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGP2017]
[GGP2017]	(Grazian+Giallongo+Paris+, 2017)
Write:	<<[GGP2017] COSMOS NNNNN>> <<[GGP2017] EGS NNNNN>> <<[GGP2017] GDN NNNNN>>
N:	2+15+2
Object:	Star-forming G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	LBT LBC deep U band observations of N=2+15+2 galaxies at z∼3.3 in the COSMOS field, the Extended Groth Strip field, and the GOODS-North field respectively. See also [BGG2011b].
in source:	NAME COSMOS Field
in source:	NAME Extended Groth Strip
in source:	NAME GOODS North Field
Ref:	=2017A&A...602A..18G
by	GRAZIAN A. , GIALLONGO E., PARIS D., BOUTSIA K., DICKINSON M., SANTINI P., WINDHORST R.A., JANSEN R.A., COHEN S.H., ASHCRAFT T.A., SCARLATA C., RUTKOWSKI M.J., VANZELLA E., CUSANO F., CRISTIANI S., GIAVALISCO M., FERGUSON H.C., KOEKEMOER A., GROGIN N.A., CASTELLANO M., FIORE F., FONTANA A., MARCHI F., PEDICHINI F., PENTERICCI L., AMORIN R., BARRO G., BONCHI A., BONGIORNO A., FABER S.M., FUMANA M., GALAMETZ A., GUAITA L., KOCEVSKI D.D., MERLIN E., NONINO M., O'CONNELL R.W., PILO S., RYAN R.E., SANI E., SPEZIALI R., TESTA V., WEINER B., YAN H.
	Astron. Astrophys., 602A, 18-18 (2017)
	Lyman continuum escape fraction of faint galaxies at z ~ 3.3 in the CANDELS/GOODS-North, EGS, and COSMOS fields with LBC.
o	Table 1: <[GGP2017] COSMOS NNNNN> (Nos 53167, 59330), <[GGP2017] EGS NNNNN> N=15 among (Nos 724-14043), <[GGP2017] GDN NNNNN> (Nos 91000, 91200).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGP88]
[GGP88]	(Green+Godwin+Peach, 1988)
Write:	<<[GGP88] Cl 2354-35 X>> <<[GGP88] HHMM+DD>> <<[GGP88] HHMM+DD N>> <<[GGP88] ACO 496 N>> <<[GGP88] Pavo Group X>> <<[GGP88] Klem 2 NN>>
N:	1+7+3+1+6
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table 2: galaxies in southern clusters. The numbering system for clusters Ser 40-6, Klem 44 and ClG 2354-35 are those used in [GGP90] (in prepa in 1988). Format 'HHMM+DD' and 'HHMM+DD N' are used for galaxies near ClG 2354-35.
in source:	ClG 2354-35
in source:	ACO 496
in source:	NAME PAVO GROUP
in source:	Klem 2
Ref:	=1988MNRAS.234.1051G
by	GREEN M.R. , GODWIN J.G., PEACH J.V.
	Mon. Not. R. Astron. Soc., 234, 1051-1058 (1988)
	Redshifts of galaxies in some southern groups and clusters.
o	Table 2, col(1): [GGP90] Klem 44 NN, [GGP90] Ser 40-6 NN, [GGP90] Cl 2354-35 NN.
o	Table 2: <[GGP88] Cl 2354-35 X> N=1, <[GGP88] HHMM-DD> N=5, <[GGP88] 2347-36 N> (Nos 1-2), <[GGP88] ACO 496 N> (Nos 1, 7, 8), <[GGP88] Pavo Group X> N=1, <[GGP88] Klem 2 NN> N=6 among (Nos 9-21).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGP90]
[GGP90]	(Green+Godwin+Peach, 1990)
Write:	<<[GGP90] Klem 44 NNN>> <<[GGP90] Ser 40-6 NNN>> <<[GGP90] Cl 2354-35 NNN>>
N:	507+481+284
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	G in 3 ClG: Klem 44, Ser 40-6 and ClG 2354-35 (= ACO 4059). The numbering for these 3 clusters was already used in [GGP88].
in source:	Klem 44
in source:	Ser 40-6 = ACO 3266
in source:	ClG 2354-35
Ref:	=1990MNRAS.243..159G
by	GREEN M.R. , GODWIN J.G., PEACH J.V.
	Mon. Not. R. Astron. Soc., 243, 159-170 (1990)
	Three southern cD clusters of galaxies Klemola 44, Sersic 40/6 and 2354-35.
o	Microfiche: <[GGP90] Klem 44 NNN> (Nos 1-507), <[GGP90] Ser 40-6 NNN> (Nos 1-481), <[GGP90] Cl 2354-35 NNN> (Nos 1-284).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GGPFH
GGPFH	(Goetz+Gutermuth+Pipher+Forrest+Howard) (Not yet in Simbad)
Write:	<<GGPFH N>>
N:	1
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	One new compact object with Br-alpha emission is seen by the authors.
Ref:	=2003ApJ...599.1173G
by	GOETZ J.A. , GUTERMUTH R., PIPHER J.L., FORREST W.J., HOWARD E.M.
	Astrophys. J., 599, 1173-1188 (2003)
	The compact H II region S88B: excitation and extinction.
o	Text: <GGPFH N> (No. 1).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GGR
GGR	(Gonzalez+Gonzalez, direction of the gal. Rotation)= (3G) = (G-G)
Write:	<<*Em GGR** NNN>>
N:	212
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Ref:	=1956BOTT....2o..16G
by	GONZALEZ G. , GONZALEZ G.
	Bol. Obs. Tonantz. Tacub., 2, part no 15, 16-26 (1956)
	Estrellas con Hα en emission en las longitudes galacticas de 59 a 90 °.
o	At the end of Table 1 (page 26), the hours of RA are 0h and 1h (not 23h as indicated on the top lines)
o	Table I: <EM* GGR NNN> (Nos 1-212)
Details on Acronym: [GGR2006]
[GGR2006]	(Geha+Guhathakurta+Rich+, 2006)
Write:	<<[GGR2006] NNNNNN>>
N:	725
Object:	* (SIMBAD class: Star)
Note:	Keck DEIMOS spectroscopic observations of NGC 205. See also [DBL2003].
in source:	NGC 205 = M 110
Ref:	=2006AJ....131..332G
by	GEHA M. , GUHATHAKURTA P., RICH R.M., COOPER M.C.
	Astron. J., 131, 332-342 (2006)
	Local Group dwarf elliptical galaxies. I. Mapping the dynamics of NGC 205 beyond the tidal radius.
o	Table 3: NGC 205 star designation are not '[DBL2003] NNN'.
o	Table 3: <[GGR2006] NNNNNN> N=725 among (Nos 2186-127882).
=E=	Catalogue in electronic form as J/AJ/131/332
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGR2014]
[GGR2014]	(Guzman+Garay+Rodriguez+, 2014)
Write:	<<[GGR2014] NN>>
N:	18
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA 92GHz observations of N=18 continuum sources in the field of MSX6C G345.4938+01.4677.
Ref:	=2014ApJ...796..117G
by	GUZMAN A.E. , GARAY G., RODRIGUEZ L.F., MORAN J., BROOKS K.J., BRONFMAN L., NYMAN L.-A., SANHUEZA P., MARDONES D.
	Astrophys. J., 796, 117 (2014)
	The slow ionized wind and rotating disklike system that are associated with the high-mass young stellar object G345.4938+01.4677.
o	Fig. 1, Table 2: <[GGR2014] NN> (Nos 1-18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGR2016]
[GGR2016]	(Guzman+Garay+Rodriguez+, 2016)
Write:	<<[GGR2016] W1>> <<[GGR2016] N>>
N:	1+3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA observations at 5, 9, 17 and 19GHz of N=1+3 radio sources in the field of MSX6C G345.4938+01.4677.
in source:	IRAS 16562-3959 = MSX6C G345.4938+01.4677
Ref:	=2016ApJ...826..208G
by	GUZMAN A.E. , GARAY G., RODRIGUEZ L.F., CONTRERAS Y., DOUGADOS C., CABRIT S.
	Astrophys. J., 826, 208-208 (2016)
	A protostellar jet emanating from a hypercompact H II region.
o	Fig. 1, Tables 2-3: <[GGR2016] W1> N=1, <[GGR2016] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGR94]
[GGR94]	(Ghosh+Gopal-Krishna+Rao, 1994)
Write:	<<[GGR94] HHMM+DDd>>
N:	46
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Ref:	=1994A&AS..106...29G
by	GHOSH T. , GOPAL-KRISHNA, RAO A.P.
	Astron. Astrophys., Suppl. Ser., 106, 29-37 (1994)
	Three-year monitoring of a sample of flat-spectrum radio sources at 327 MHz.
o	Table 2 not in Simbad, except 3C sources
o	Table 1: <[GGR94] HHMM+DDd> N=46
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGS2000]
[GGS2000]	(Gopal-Krishna+Gupta+Sagar+, 2000) (Not yet in Simbad)
Write:	<<[GGS2000] HHMM+DDd>> <<[GGS2000] Star N>>
N:	1+5
Object:	QSO + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	One QSO is new '0824+098'. N=5 comparison stars for the QSOs.
Ref:	=2000MNRAS.314..815G
by	GOPAL-KRISHNA , GUPTA A.C., SAGAR R., WIITA P.J., CHAUBEY U.S., STALIN C.S.
	Mon. Not. R. Astron. Soc., 314, 815-825 (2000)
	Rapid optical variability in radio-quiet QSOs.
o	Table 2: <[GGS2000] Star N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGS2012]
[GGS2012]	(Gettings+Gonzalez +Stanford+, 2012)
Write:	<<[GGS2012] JHHMMSS.ss+DDMMSS.s>>
N:	12
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Subaru MOIRCS (J and Ks) and Keck LRIS spectroscopy of N=12 galaxies in the field of the galaxy cluster MOO J2342.0+1301. See also [GDB2015] and [GGB2019].
in source:	MOO J2342.0+1301
Ref:	=2012ApJ...759L..23G
by	GETTINGS D.P. , GONZALEZ A.H., STANFORD S.A., EISENHARDT P.R.M., BRODWIN M., MANCONE C., STERN D., ZEIMANN G.R., MASCI F.J., PAPOVICH C., TANAKA I., WRIGHT E.L.
	Astrophys. J., 759L, 23 (2012)
	The Massive Distant Clusters of WISE Survey: the first distant galaxy cluster discovered by WISE.
o	<MOO J2342.0+1301> N=1. Table 1: <[GGS2012] JHHMMSS.ss+DDMMSS.s> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGS2018]
[GGS2018]	(Greco+Greene+Strauss+, 2018)
Write:	<<[GGS2018] NNN>>
N:	781
Object:	LSB (SIMBAD class: LowSurfBrghtG = Low Surface Brightness Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Identification of N=781 low surface brightness galaxies. Use of the Wide layer of the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) imaging survey of 200 deg^2.
Ref:	=2018ApJ...857..104G
by	GRECO J.P. , GREENE J.E., STRAUSS M.A., MACARTHUR L.A., FLOWERS X., GOULDING A.D., HUANG S., KIM J.H., KOMIYAMA Y., LEAUTHAUD A., LEISMAN L., LUPTON R.H., SIFON C., WANG S.-Y.
	Astrophys. J., 857, 104-104 (2018)
	Illuminating low surface brightness galaxies with the Hyper Suprime-Cam survey.
o	Table 1: <[GGS2018] NNN> (Nos 1-781).
=E=	Catalogue in electronic form as J/ApJ/857/104
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGS97]
[GGS97]	(Galama+Groot+Strom+, 1997)
Write:	<<[GGS97] JHHMM.m+DDMM>>
N:	3
Object:	G + (Rad) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Radio observations with the IPN WGC of the error box of GRB 970111. p.7: N=1 galaxy, 'J1528.2+1935'. p.8: N=2 radio-sources, 'J1528.2+1933' and 'J1528.1+1935'.
Ref:	=1997ApJ...486L...5G
by	GALAMA T.J. , GROOT P.J., STROM R.G., VAN PARADIJS J., HURLEY K., KOUVELIOTOU C., FISHMAN G.J., MEEGAN C.A., HEISE J., IN'T ZAND J.J.M., DE BRUYN A.G., HANLON L.O., BENNETT K., TELTING J.H., RUTTEN R.G.M.
	Astrophys. J., 486, 5-10 (1997)
	Radio and optical follow-up observations and improved interplanetary network position of GRB 970111.
o	p.7, 8: <[GGS97] JHHMM.m+DDMM> N=3
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GGSS
GGSS	(Grid Giant Star Survey)
Write:	<<GGSS JHHMMSS.ss+DDMMSS.s>> <<GGSS JHHMMSS.s+DDMMSS>>
N:	8+434+341+183
Object:	* (SIMBAD class: Star)
Note:	2002ApJ...576L.125K: 1st ref. with 'GGSS' stars. Table 1, col. Name: the format JHHMM+DD.NNN will not be used in the final GGSS catalogue, but the authors will use the format JHHMMSS.ss+DDMMSS.s (email discussion with A. KUNDU).
Ref:	=2002ApJ...576L.125K
by	KUNDU A. , MAJEWSKI S.R., RHEE J., ROCHA-PINTO H.J., POLAK A.A., SLESNICK C.L., KUNKEL W.E., JOHNSTON K.V., PATTERSON R.J., GEISLER D., GIEREN W., SEGUEL J.C., SMITH V.V., PALMA C., ARENAS J., CRANE J.D., HUMMELS C.B.
	Astrophys. J., 576, 125-129 (2002)
	Exploring halo substructure with giant stars. III. First results from the grid giant star survey and discovery of a possible nearby Sagittarius tidal structure in Virgo.
o	Table 1, col. Name: the format JHHMM+DD.NNN will not be used in the final GGSS catalogue, but Authors will use the format JHHMMSS.ss+DDMMSS.s (email discussion with A. KUNDU).
o	Table 1: <GGSS JHHMMSS.ss+DDMMSS.s> N=8.
Ref:	=2006AJ....131.1784B
by	BIZYAEV D. , SMITH V.V., ARENAS J., GEISLER D., MAJEWSKI S.R., PATTERSON R.J., CUNHA K., DEL PARDO C., SUNTZEFF N.B., GIEREN W.
	Astron. J., 131, 1784-1796 (2006)
	The Space Interferometry Mission Astrometric Grid Giant Star Survey. I. Stellar parameters and radial velocity variability.
o	Tables 1, 6: <GGSS JHHMMSS.ss+DDMMSS.s> N=434+341).
Ref:	=2010AJ....140.1911B
by	BIZYAEV D. , SMITH V.V., CUNHA K.
	Astron. J., 140, 1911-1918 (2010)
	The Space Interferometry Mission Astrometric Grid Giant Star Survey. III. Basic stellar parameters for an extended sample.
o	Table 3: <GGSS JHHMMSS.s+DDMMSS> N=183.
=E=	Catalogue in electronic form as <J/AJ/131/1784/>
=E=	Catalogue in electronic form as <J/AJ/140/1911/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GGT2003]
[GGT2003]	(Giroletti+Giovannini+Taylor+, 2003) (Not yet in Simbad)
Write:	<<[GGT2003] 4C 31.04 WN>>
N:	3+9
Object:	Component (SIMBAD class: Radio = Radio Source)
in source:	4C 31.04
Ref:	=2003A&A...399..889G
by	GIROLETTI M. , GIOVANNINI G., TAYLOR G.B., CONWAY J.E., LARA L., VENTURI T.
	Astron. Astrophys., 399, 889-897 (2003)
	Lobe advance velocities in the extragalactic compact symetric object 4C 31.04.
o	parag. 2.1: calibrator J0423-1020 not identified.
o	Fig.3, Table 1: <[GGT2003] 4C 31.04 W> (Nos E, W, C), <[GGT2003] 4C 31.04 WN> (Nos W1-W3, E1-E6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGV2016]
[GGV2016]	(Gomez-Guijarro+Gallego+Villar+, 2016)= HAWKI
Write:	<<[GGV2016] HAWKI000NNNN>>
N:	4
Object:	Poss. Em. Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	VLT HAWK-I observations of N=4 candidate emission-line emitters in the GOODS South field.
in source:	NAME GOODS South Field
Ref:	=2016A&A...591A.151G
by	GOMEZ-GUIJARRO C. , GALLEGO J., VILLAR V., RODRIGUEZ-MUNOZ L., CLEMENT B., CUBY J.-G.
	Astron. Astrophys., 591A, 151-151 (2016)
	Properties of galaxies at the faint end of the Hα luminosity function at z ~ 0.62.
o	Table A.1: <[GGV2016] HAWKI000NNNN> (Nos 3148, 3151, 3361, 3606).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GGV99]
[GGV99]	(Gaensler+Gotthelf+Vasiht, 1999)
Write:	<<[GGV99] JHHMMSS.ss+DDMMSS.s>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=2 point sources in the field of PSR J1845-0258.
Ref:	=1999ApJ...526L..37G
by	GAENSLER B.M. , GOTTHELF E.V., VASISHT G.
	Astrophys. J., 526, 37-40 (1999)
	A new supernova remnant coincident with the slow X-ray pulsar AX J1845-0258.
o	PSR J1845-0258 = AX J1844.8-0258.
o	p.38: <[GGV99] JHHMMSS.ss-DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GH
GH	(Gurwell+Hodge)
Write:	<<GH FF-NN>>
N:	96
Object:	G (SIMBAD class: Galaxy)
Note:	List of 96 galaxies brigter than V = 16.5, seen through the LMC. In the format 'FF' stands for fields (Nos 1-11), object 'GH 2-3' is missing.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1990PASP..102..849G
by	GURWELL M. , HODGE P.
	Publ. Astron. Soc. Pac., 102, 849-853 (1990)
	Galaxies behind the Large Magellanic Cloud.
o	Table 3: <GH FF-NN> N=96
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GH
GH	(Greene+Ho)
*****	Avoid the usage of GH, prefer [GH2004]
Origin	of the Acronym: L (2008ApJ...686..838W)
Details on Acronym: GH
GH	(Graham+Heyer)
*****	Avoid the usage of GH, prefer [GH90b]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: GH
GH	(Geller+Huchra)
*****	Avoid the usage of GH, prefer GHCG
Origin	of the Acronym: L = Found in the literature
Details on Acronym: GH
GH	(Giclas, Hyades)
*****	Avoid the usage of GH, prefer HG
Details on Acronym: [GH2004]
[GH2004]	(Greene+Ho, 2004)= (GH)
Write:	<<[GH2004] NN>>
N:	19
Object:	Poss. Black Hole (SIMBAD class: AGN = Active Galaxy Nucleus)
Stat:	is completely incorporated in Simbad
Note:	Initial sample of 19 intermediate-mass black hole candidates in active galactic nuclei from the first data release of the SDSS.
Ref:	=2004ApJ...610..722G
by	GREENE J.E. , HO L.C.
	Astrophys. J., 610, 722-736 (2004)
	Active galactic nuclei with candidate intermediate-mass black holes.
o	Table 1: <[GH2004] NN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GH2008]
[GH2008]	(Gotthelf+Halpern, 2008)
Write:	<<[GH2008] NN>>
N:	18
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS observations of the field of HESS J1837-069.
Ref:	=2008ApJ...681..515G
by	GOTTHELF E.V. , HALPERN J.P.
	Astrophys. J., 681, 515-521 (2008)
	Discovery of a young, energetic 70.5 ms pulsar associated with the TeV γ-ray source HESS J1837-069.
o	Fig.1, Table 1: <[GH2008] NN> (Nos 1-18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GH2013]
[GH2013]	(Gao+Han, 2013)= ([GH2013a])
Write:	<<[GH2013] G195.60-02.95>>
N:	1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=1 probable HII region in the Origem Loop. Use of multi-frequency radio survey data.
in source:	NAME Origem Loop
Ref:	=2013A&A...551A..16G
by	GAO X.Y. , HAN J.L.
	Astron. Astrophys., 551A, 16-16 (2013)
	The Origem Loop.
o	Text: <[GH2013] G195.60-02.95> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GH2013a]
[GH2013a]	(Gao+Han, 2013)
*****	Avoid the usage of [GH2013a], prefer [GH2013]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GH2013b]
[GH2013b]	(Grammer+Humphreys, 2013)
Write:	<<[GH2013b] JHHMMSS.ss+DDMMSS.ss>>
N:	539825
Object:	* (SIMBAD class: Star)
Note:	BVI photometric catalog of N=539825 luminous stars in M101. Use of archival HST/ACS WFC images.
in source:	M 101 = NGC 5457
Ref:	=2013AJ....146..114G
by	GRAMMER S. , HUMPHREYS R.M.
	Astron. J., 146, 114 (2013)
	The massive star population in M101. I. The identification and spatial distribution of the visually luminous stars.
o	Table 2: <[GH2013b] JHHMMSS.ss+DDMMSS.ss> N=539825.
=E=	Catalogue in electronic form as <J/AJ/146/114/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GH2015]
[GH2015]	(Gutermuth+Heyer, 2015)
Write:	<<[GH2015] MG GLLL.llll+BB.bbbb>> <<[GH2015] MGLLL.llll+BB.bbbb>> (not recognised by Simbad, but found in literature)
N:	933818+419410
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	24µm based point source catalog derived from the image data of the MIPSGAL 24µm Galactic Plane Survey (MIPSGAL) and the corresponding data products. The high quality catalog product contains 933918 sources, with a total of 1353228 in the full archive catalog.
Ref:	=2015AJ....149...64G
by	GUTERMUTH R.A. , HEYER M.
	Astron. J., 149, 64 (2015)
	A 24µm point source catalog of the galactic plane from Spitzer/MIPSGAL.
o	catalog.dat, archive.dat: <[GH2015] MG GLLL.llll+BB.bbbb> N=933818+419410.
=E=	Catalogue in electronic form as J/AJ/149/64
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GH2O
GH2O	(Gal. H2O em. source)= (H2O)
Write:	<<GH2O LLL.ll+BB.bb>>
Object:	Gal. Maser + MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	Systematic designation
Auth.:	CESARONI R.+
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GH77]
[GH77]	(Giovanelli+Haynes, 1977)
Write:	<<[GH77] NN>>
N:	12
Object:	Cloudet (SIMBAD class: Cloud)
in source:	[H68] A
Ref:	=1977A&A....54..909G
by	GIOVANELLI R. , HAYNES M.P.
	Astron. Astrophys., 54, 909-913 (1977)
	Fine structure in high velocity H I gas.
o	Table 1: <[GH77] NN> (Nos 1-12)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GH90]
[GH90]	(Gyulbudaghian+Hakopian, 1990)
====>	Equivalent to: [GA90]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GH90b]
[GH90b]	(Graham+Heyer, 1990)= (GH)
Write:	<<[GH90b] NNW>>
N:	12
Object:	Em. Obj. (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-10) in the 1st ref. Nos 10W and 10E are added in the 2nd ref.
in source:	LDN 1551
Ref:	=1990PASP..102..972G
by	GRAHAM J.A. , HEYER M.H.
	Publ. Astron. Soc. Pac., 102, 972-977 (1990)
	New optical features in L 1551 and HH 30.
o	<[GH90b] NN> (Nos 1-10)
Ref:	=1992RMxAA..24...99G
by	GARNAVICH P.M. , NORIEGA-CRESPO A., GREEN P.J.
	Rev. Mex. Astron. Astrofis., 24, 99-107 (1992)
	Wide field imaging of the star forming region Lynds 1551.
o	Table 1: <[GH90b] NNW> Nos 10W and 10E. Table 2: <[GNG92] NNA> (Nos 1-25), N=34
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GH91]
[GH91]	(Gudehus+Hegyi, 1991)
Write:	<<[GH91] NNN>>
N:	213
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=213: 203 G + 10 *
in source:	ACO 1689
Ref:	=1991AJ....101...18G
by	GUDEHUS D.H. , HEGYI D.J.
	Astron. J., 101, 18-56 (1991)
	Two-band CCD surface photometry of cluster Abell 1689.
o	<[GH91] NNN> N=213
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GH93]
[GH93]	(Giovanelli+Haynes, 1993)= ([GH93a])
Write:	<<[GH93] HHMMSS.s+DDMMSS>>
N:	765
Object:	G in Supercluster (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	NAME PPS
Ref:	=1993AJ....105.1271G
by	GIOVANELLI R. , HAYNES M.P.
	Astron. J., 105, 1271-1290 (1993)
	A survey of the Pisces-Perseus supercluster. VI. The declination zone +15.5°. to +21.5°.
o	Table 1: <[GH93] HHMMSS.s+DDMMSS> N=765
=E=	Catalogue in electronic form as J/AJ/105/1271
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GH93a]
[GH93a]	(Giovanelli+Haynes, 1993)
*****	Avoid the usage of [GH93a], prefer [GH93]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GH93b]
[GH93b]	(Gibb+Heaton, 1993)
Write:	<<[GH93b] A>> <<[GH93b] A'>>
N:	6+4
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Note:	(Nos A-F), 6 HCO+ clumps in HH 24-26 region. (Nos A', B', E', F'), 4 CS clumps in HH 24-26 region.
in source:	NAME HH 24-26
Ref:	=1993A&A...276..511G
by	GIBB A.G. , HEATON B.D.
	Astron. Astrophys., 276, 511-521 (1993)
	The star-forming region around HH 24-26 : a revised morphology.
o	Table 3, Fig.5: <[GH93b] A> (Nos A-F). Table 4, Fig.7: <[GH93b] A'> (Nos A', B', E', F').
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GH96]
[GH96]	(Greiner+Hazen, 1996)
Write:	<<[GH96] N>>
N:	9
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Stellar objects within the X-ray error circle of RX J0527.8-6954. See also ref. 1997MNRAS.291L..13A
Ref:	=1996IBVS.4409....1G
by	GREINER J. , HAZEN M.L.
	IAU Inform. Bull. Var. Stars, 4409, 1-4 (1996)
	HV 2554 and the supersoft X-ray source RX J0527.8-6954.
o	Fig. 2: <[GH96] N> (Nos 1-9)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHA2004]
[GHA2004]	(Georgakakis+Hopkins+Afonso+, 2004)
Write:	<<[GHA2004] NN>>
N:	43
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Radio properties of hard X-ray selected sources by combining XMM-Newton pointing with the Phoenix Deep Survey (see PDF).
Ref:	=2004MNRAS.354..127G
by	GEORGAKAKIS A. , HOPKINS A.M., AFONSO J., SULLIVAN M., MOBASHER B., CRAM L.E.
	Mon. Not. R. Astron. Soc., 354, 127-141 (2004)
	The Phoenix Deep Survey: the radio properties of the hard X-ray-selected sample.
o	Table 1: <[GHA2004] NN> (Nos 1-43).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHA2006]
[GHA2006]	(Georgakakis+Hopkins+Afonso+, 2006)
Write:	<<[GHA2006] NN>>
N:	17
Object:	Extremely Red Obj. (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Phoenix Deep Survey: search for Extremely Red Objects from deep multicolour imaging using the Wide Field Imager at the AAT.
Ref:	=2006MNRAS.367..331G
by	GEORGAKAKIS A. , HOPKINS A.M., AFONSO J., SULLIVAN M., MOBASHER B., CRAM L.E.
	Mon. Not. R. Astron. Soc., 367, 331-338 (2006)
	The Phoenix Deep Survey: the star formation rates and the stellar masses of extremely red objects.
o	Table 1: <[GHA2006] NN> (Nos 1-17).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHB2000]
[GHB2000]	(Gomez+Hughes+Birkinshaw, 2000)
Write:	<<[GHB2000] NNN>>
N:	147
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=147 objects in the field of ACO 665. Among them, 77 are confirmed cluster members.
in source:	ACO 665
Ref:	=2000ApJ...540..726G
by	GOMEZ P.L. , HUGHES J.P., BIRKINSHAW M.
	Astrophys. J., 540, 726-740 (2000)
	A merger scenario for the dynamics of Abell 665.
o	Table 2: <[GHB2000] NNN> (Nos 1-147).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHB2007]
[GHB2007]	(Groppi+Hunter+Blundel+, 2007)= (I) = (IRAC) = (SMA)
Write:	<<[GHB2007] SMA N>> <<[GHB2007] I NN>>
N:	2+10
Object:	(smm) + (IR) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Multiwavelength images of the R CrA molecular cloud: N=2 SMA 1.1mm continuum sources, and N=10 Spitzer IRAC sources.
in source:	NAME R CrA Cloud
Ref:	=2007ApJ...670..489G
by	GROPPI C.E. , HUNTER T.R., BLUNDELL R., SANDELL G.
	Astrophys. J., 670, 489-498 (2007)
	High spatial resolution observations of two young protostars in the R Corona Australis region.
o	SMM N Table 2 = [NWA2005] SMM N in Simbad.
o	Fig.1, Table 1: <[GHB2007] SMA N> (Nos 1-2). Table 3: <[GHB2007] I NN> (Nos 1-10). Table 2, first col.: <[NWA2005] SMM 1A S> N=1 added. Table 2, last col.: <vdA N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHB2017]
[GHB2017]	(Garcia-Vergara+Hennawi+Barrientos+, 2017)
Write:	<<[GHB2017] SDSSJHHMM+DDMM NN>> <<[GHB2017] J2003-3300 1>>
N:	43+1
Object:	LBG (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	VLT FORS1 observations of N=43+1 Lyman Break Galaxies (LBGs) in the fields of six QSOs.
Ref:	=2017ApJ...848....7G
by	GARCIA-VERGARA C. , HENNAWI J.F., BARRIENTOS L.F., RIX H.-W.
	Astrophys. J., 848, 7-7 (2017)
	Strong clustering of Lyman Break galaxies around luminous quasars at z ~ 4.
o	Table 3: <[GHB2017] SDSSJHHMM+DDMM NN> N=37, <[GHB2017] J2003-3300 1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHB2019]
[GHB2019]	(Garcia-Vergara+Hennawi+Barrientos+, 2019)
Write:	<<[GHB2019] SDSS JHHMM+DDMM N>> <<[GHB2019] SDSS JHHMM+DDMM_N>> (not recognised by Simbad, but found in literature)
N:	25
Object:	Poss. LAE (SIMBAD class: EmObj = Emission Object)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 narrow-band observations of N=25 LAE (Lyman Alpha Emitters) candidates in the field of 11 QSOs.
Ref:	=2019ApJ...886...79G
by	GARCIA-VERGARA C. , HENNAWI J.F., BARRIENTOS L.F., ARRIGONI BATTAIA F.
	Astrophys. J., 886, 79-79 (2019)
	Clustering of Lyα emitters around quasars at z ~ 4.
o	Table 3: <[GHB2019] SDSS JHHMM+DDMM N> N=25.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHC2009]
[GHC2009]	(Gezari+Heckman+Cenko+, 2009)
Write:	<<[GHC2009] D23H-1>>
N:	1
Object:	Tidal disruption event candidate (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	N=1 candidate tidal disruption event in the GALEX Deep Imaging Survey.
Ref:	=2009ApJ...698.1367G
by	GEZARI S. , HECKMAN T., CENKO S.B., ERACLEOUS M., FORSTER K., GONCALVES T.S., MARTIN D.C., MORRISSEY P., NEFF S.G., SEIBERT M., SCHIMINOVICH D., WYDER T.K.
	Astrophys. J., 698, 1367-1379 (2009)
	Luminous thermal flares from quiescent supermassive black holes.
o	Text: <[GHC2009] D23H-1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHC2010]
[GHC2010]	(Goodger+Hardcastle+Croston+, 2010)= ([GHC2010a]) (Not yet in Simbad)
Write:	<<[GHC2010] ANA>> <<[GHC2010] SJN>> <<[GHC2010] SN>> <<[GHC2010] SNA>> <<[GHC2010] AXNA>>
N:	19+13
Object:	Radio knot + X-ray knot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT observations of the jet of Centaurus A. Use of archival Chandra data.
in source:	Cen A = NGC 5128
Ref:	=2010ApJ...708..675G
by	GOODGER J.L. , HARDCASTLE M.J., CROSTON J.H., KRAFT R.P., BIRKINSHAW M., EVANS D.A., JORDAN A., NULSEN P.E.J., SIVAKOFF G.R., WORRALL D.M., BRASSINGTON N.J., FORMAN W.R., GILFANOV M., JONES C., MURRAY S.S., RAYCHAUDHURY S., SARAZIN C.L., VOSS R., WOODLEY K.A.
	Astrophys. J., 708, 675-697 (2010)
	Long-term monitoring of the dynamics and particle acceleration of knots in the jet of Centaurus A.
o	Fig. 1, Tables 5-7: <[GHC2010] ANA>, <[GHC2010] SJN>, <[GHC2010] SNA>, N=19. Fig. 2, Tables 3+5+7: <[GHC2010] AXNA> N=13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHC2010a]
[GHC2010a]	(Goodger+Hardcastle+Croston+, 2010) (Not yet in Simbad)
*****	Avoid the usage of [GHC2010a], prefer [GHC2010]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHC2010b]
[GHC2010b]	(Garcia+Herrero+Castro+, 2010) (Not yet in Simbad)
Write:	<<[GHC2010b] NNN>>
Object:	OB Assoc. (SIMBAD class: Association = Association of Stars)
Note:	N=166 OB associations in IC 1613.
in source:	IC 1613
Ref:	=2010A&A...523A..23G
by	GARCIA M. , HERRERO A., CASTRO N., CORRAL L., ROSENBERG A.
	Astron. Astrophys., 523A, 23-23 (2010)
	The young stellar population of IC 1613. II. Physical properties of OB associations.
o	Table 1: <[GHC2010b] NNN> N=166 among (Nos 2-197). Table 4: <[GHV2009] Star NNNN> N=13 among (Nos 52443-75661).
=E=	Catalogue in electronic form as <J/A+A/523/A23/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GHCG
GHCG	(Geller+Huchra, Cluster of G)= (CfA) = (GH)
Write:	<<GHCG NNN>>
N:	176
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Ref:	=1983ApJS...52...61G
by	GELLER M.J. , HUCHRA J.P.
	Astrophys. J., Suppl. Ser., 52, 61-87 (1983)
	Groups of galaxies. III. THe CfA survey.
o	(Erratum) + erratum Vol 54, 442
o	Table 1: <GHCG NNN> (Nos 1-176)
=E=	Catalogue in electronic form as VII/84
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [GHD2014]
[GHD2014]	(Geller+Hwang+Diaferio+, 2014)
Write:	<<[GHD2014] NNNN>>
N:	2510
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	MMT 6.5m telescope Hectospec spectroscopic observations of N=2510 galaxies in the region around A383.
in source:	ACO 383
Ref:	=2014ApJ...783...52G
by	GELLER M.J. , HWANG H.S., DIAFERIO A., KURTZ M.J., COE D., RINES K.J.
	Astrophys. J., 783, 52 (2014)
	A redshift survey of the strong-lensing cluster Abell 383.
o	Table 1: <[GHD2014] NNNN> (Nos 1-2510).
=E=	Catalogue in electronic form as J/ApJ/783/52
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHE2001]
[GHE2001]	(Grindlay+Heinke+Edmonds, 2001)= ([GHE2001a])
Write:	<<[GHE2001] WNNN>>
N:	108+15+180+81
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS-I and extensive HST WFPC2 study of X-ray sources in 47 Tuc.
in source:	NGC 104 = 47 Tuc
Ref:	=2001Sci...292.2290G
by	GRINDLAY J.E. , HEINKE C., EDMONDS P.D., MURRAY S.S.
	Science, 292, 2290-2295 (2001)
	High-resolution X-ray imaging of a globular cluster core: compact binaries in 47 Tuc.
o	Fig.1: XNN = [HJV94] NN. E8 = Cl* NGC 104 EGG V8. AKO9 = Cl* NGC 104 AKO 9. A = PSR 0021-72A (Nos among C to Q).
o	Catalogue: <[GHE2001] WNNN> (Nos W1-W108).
Ref:	=2003ApJ...596.1177E
by	EDMONDS P.D. , GILLILAND R.L., HEINKE C.O., GRINDLAY J.E.
	Astrophys. J., 596, 1177-1196 (2003)
	An extensive census of Hubble Space Telescope counterparts to Chandra X-ray sources in the globular cluster 47 Tucanae. I. Astrometry and photometry.
o	Tables 1, 4: <[GHE2001] WNNN> N=16 added among (Nos W115-W184). Fig.7: <Cl* NGC 104 EGH RN> (Nos R1-R2).
Ref:	=2005ApJ...625..796H
by	HEINKE C.O. , GRINDLAY J.E., EDMONDS P.D., COHN H.N., LUGGER P.M., CAMILO F., BOGDANOV S., FREIRE P.C.
	Astrophys. J., 625, 796-824 (2005)
	A deep Chandra survey of the globular cluster 47 Tucanae: catalog of point sources.
o	Table 2: <[GHE2001] WNNN> N=180 added among (Nos W113-W351). Table 2: <CXOGlb JHHMMSS.s+DDMMSS> N=300.
Ref:	=2017MNRAS.472.3706B
by	BHATTACHARYA S. , HEINKE C.O., CHUGUNOV A.I., FREIRE P.C.C., RIDOLFI A., BOGDANOV S.
	Mon. Not. R. Astron. Soc., 472, 3706-3721 (2017)
	Chandra studies of the globular cluster 47 Tucanae: a deeper X-ray source catalogue, five new X-ray counterparts to millisecond radio pulsars and new constraints to r-mode instability window.
o	Table 2: <[GHE2001] WNNN> (Nos 352-432) added.
=E=	Catalogue in electronic form as J/other/Sci/292.2290
=E=	Catalogue in electronic form as J/ApJ/625/796
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHE2001a]
[GHE2001a]	(Grindlay+Heinke+Edmonds, 2001)
Note:	Chandra X-ray sources in 47 Tuc
*****	Avoid the usage of [GHE2001a], prefer [GHE2001]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHE2001b]
[GHE2001b]	(Grindlay+Heinke+Edmonds, 2001)
Write:	<<[GHE2001b] UNNN>>
N:	25+79
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra X-ray sources in NGC 6397.
in source:	NGC 6397
Ref:	=2001ApJ...563L..53G
by	GRINDLAY J.E. , HEINKE C.O., EDMONDS P.D., MURRAY S.S., COOL A.M.
	Astrophys. J., 563, 53-56 (2001)
	Chandra exposes the core-collapsed globular cluster NGC 6397.
o	Table 1: cross-id. CVN (N 1-3) = [CGC95] N, PC-N = CL* NGC 6397 PCBY N. Reference TGE01 is 2001, ApJ Let. v.553, p. 169 (and not ApJ).
o	Table 1: <[GHE2001b] UNN> N=25 among (Nos U5-U61).
Ref:	=2010ApJ...709..241B
by	BOGDANOV S. , VAN DEN BERG M., HEINKE C.O., COHN H.N., LUGGER P.M., GRINDLAY J.E.
	Astrophys. J., 709, 241-250 (2010)
	A Chandra X-ray observatory study of PSR J1740-5340 and candidate millisecond pulsars in the globular cluster NGC 6397.
o	Table 3: <[GHE2001b] UNNN> N=79 among (Nos U5-U123).
=E=	Catalogue in electronic form as <J/ApJ/709/241/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHG2001]
[GHG2001]	(Gelatt+Hunter+Gallagher, 2001)
Write:	<<[GHG2001] NN>>
N:	61
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations and near-IR ground-based spectroscopy.
in source:	NGC 4449
Ref:	=2001PASP..113..142G
by	GELATT A.E. , HUNTER D.A., GALLAGHER J.S.
	Publ. Astron. Soc. Pac., 113, 142-153 (2001)
	The star clusters in the irregular galaxy NGC 4449.
o	The central cluster is [GHG2001] 1.
o	Table 3: <[GHG2001] NN> (Nos 1-61).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHG2004]
[GHG2004]	(Garg+Huber+Garnavich+, 2004)
Write:	<<[GHG2004] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Cerro Tololo observations. Host galaxy of SN 2004GP.
Ref:	=2004IAUC.8450....2G
by	GARG A. , HUBER M., GARNAVICH P., CHALLIS P., STUBBS C., (The SuperMACHO Collaboration)
	IAU Circ., 8450, 2-None (2004)
	Supernova 2004gp.
o	<[GHG2004] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHG2013]
[GHG2013]	(Galametz+Hony+Galliano+, 2013)
Write:	<<[GHG2013] NNa>>
N:	27
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	Spitzer, APEX LABOCA and Herschel observations of N=24+3 regions and subregions in the massive star-forming complex LHA 120-N 158, N 159, N 160.
in source:	Magellanic Clouds:LMC:LHA 120-N 158 = LHA 120-N 158
in source:	Magellanic Clouds:LMC:LHA 120-N 159 = LHA 120-N 159
in source:	Magellanic Clouds:LMC:LHA 120-N 160 = LHA 120-N 160
Ref:	=2013MNRAS.431.1596G
by	GALAMETZ M. , HONY S., GALLIANO F., MADDEN S.C., ALBRECHT M., BOT C., CORMIER D., ENGELBRACHT C., FUKUI Y., ISRAEL F.P., KAWAMURA A., LEBOUTEILLER V., LI A., MEIXNER M., MISSELT K., MONTIEL E., OKUMURA K., PANUZZO P., ROMAN-DUVAL J., RUBIO M., SAUVAGE M., SEALE J.P., SEWILO M., VAN LOON J.Th.
	Mon. Not. R. Astron. Soc., 431, 1596-1617 (2013)
	The thermal dust emission in N158-N159-N160 (LMC) star-forming complex mapped by Spitzer, Herschel and LABOCA.
o	Fig. 9, Table 1: <[GHG2013] NNa> (Nos 1, 1a-1c, 2-24).
o	Calibrator PMN J0403-8100 (p.1599) not identified.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHG91]
[GHG91]	(Gallagher+Hunter+Gillett+, 1991)= (G91)
Write:	<<[GHG91] FIR N>> <<[GHG91] HI R>>
N:	3+3
Object:	[FIR] + HI (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	IRAS FIR observations of NGC 6822: N=3 FIR regions coinciding with HII regions, and N=3 HI regions.
in source:	NGC 6822
Ref:	=1991ApJ...371..142G
by	GALLAGHER III J.S. , HUNTER D.A., GILLETT F.C., RICE W.L.
	Astrophys. J., 371, 142-147 (1991)
	Far-infrared properties of NGC 6822.
o	Table 2, Fig.2: <[GHG91] FIR N> (Nos 1-3). Table 3: <[GHG91] HI R> (Nos I to III).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHH96]
[GHH96]	(Gotthelf+Hamilton+Helfand, 1996)
Write:	<<[GHH96] HHMMSS+DDMMSS>>
N:	42
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Observation with IPC aboard Einstein Observatory. Table 2: N=42 faint X-ray flashes, possible counterparts to gamma-ray bursts.
Ref:	=1996ApJ...466..779G
by	GOTTHELF E.V. , HAMILTON T.T., HELFAND D.J.
	Astrophys. J., 466, 779-794 (1996)
	The Einstein observatory detection of faint X-ray flashes.
o	Table 1: <[GHH96] HHMMSS+DDMMSS> N=42
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHI2008]
[GHI2008]	(Goto+Hanami+Imai+, 2008)
Write:	<<[GHI2008] JHHMMSS.s+DDMMSS>>
N:	16
Object:	Poss. Cluster of G (SIMBAD class: ClG_Candidate = Cluster of Galaxies Candidate)
Note:	AKARI observations of the North Ecliptic Pole region.
Ref:	=2008PASJ...60S.531G
by	GOTO T. , HANAMI H., IM M., IMAI K., INAMI H., ISHIGAKI T., LEE H.M., MATSUHARA H., NAKAGAWA T., OHYAMA Y., OYABU S., PEARSON C.P., TAKAGI T., WADA T.
	PASJ, 60S, 531-542 (2008)
	Galaxy clusters at 0.9 < z < 1.7 in the AKARI NEP Deep Field.
o	Table 1: <[GHI2008] JHHMMSS.s+DDMMSS> N=16.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GHISA
GHISA	(Galactic HI Self-Absorption)
Write:	<<GHISA LLL.ll+B.BB+VV>>
N:	69
Object:	HI (SIMBAD class: HI = HI (21cm) Source)
Note:	21cm line self-absorption (HISA) survey in the Canadian Galactic Plane Survey.
Ref:	=2005ApJ...626..195G
by	GIBSON S.J. , TAYLOR A.R., HIGGS L.A., BRUNT C.M., DEWDNEY P.E.
	Astrophys. J., 626, 195-213 (2005)
	A self-absorption census of cold H I clouds in the Canadian Galactic Plane Survey.
o	Table 1: <GHISA LLL.ll+B.bb+VV> N=69.
=E=	Catalogue in electronic form as J/ApJ/626/195
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GHJ2008]
[GHJ2008]	(Gallo+Homan+Tomsick, 2008)
Write:	<<[GHJ2008] NN>>
N:	28
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS observations of the field of XTE J1650-500.
Ref:	=2008ApJ...683L..51G
by	GALLO E. , HOMAN J., JONKER P.G., TOMSICK J.A.
	Astrophys. J., 683L, 51-54 (2008)
	Chandra detection of XTE J1650-500 in quiescence and the minimum luminosity of black hole X-ray binaries.
o	Table 1: <[GHJ2008] NN> (Nos 1-28).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHJ82]
[GHJ82]	(Gatley+Hyland+Jones, 1982)
Write:	<<[GHJ82] SMC N76B KN>> <<[GHJ82] LMC N159 KN>>
N:	3+6
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=3 (IR) in the SMC source N76B = 'LHA 115-N 76B' and N=6 (IR) in the LMC source N159 = 'LHA 120-N 159'. See also Paper II: [JHS86].
in source:	Magellanic Clouds:SMC:LHA 115-N 76B = LHA 115-N 76B
in source:	Magellanic Clouds:LMC:LHA 120-N 159 = LHA 120-N 159
Ref:	=1982MNRAS.200..521G
by	GATLEY I. , HYLAND A.R., JONES T.J.
	Mon. Not. R. Astron. Soc., 200, 521-526 (1982)
	Star formation in the Magellanic Clouds -II. Discovery of a protostar in the Small Magellanic Cloud.
o	Table 1: <[GHJ82] SMC N76B KN> (Nos K1-K3), <[GHJ82] LMC N159 KN> (Nos K1-K6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHK2005]
[GHK2005]	(Giovanelli+Haynes+Kent+, 2005)= (ALFALFA)
Write:	<<[GHK2005] HI JHHMMSS.s+DDMMSS>>
N:	166
Object:	HI (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	Arecibo L-band Feed Array (ALFA) receiver system observations of HI regions. See also ALFALFA.
Ref:	=2005AJ....130.2613G
by	GIOVANELLI R. , HAYNES M.P., KENT B.R., PERILLAT P., CATINELLA B., HOFFMAN G.L., MOMJIAN E., ROSENBERG J.L., SAINTONGE A., SPEKKENS K., STIERWALT S., BROSCH N., MASTERS K.L., SPRINGOB C.M., KARACHENTSEV I.D., KARACHENTSEVA V.E., KOOPMANN R.A., MULLER E., VAN DRIEL W., VAN ZEE L.
	Astron. J., 130, 2613-2624 (2005)
	The Arecibo Legacy Fast ALFA survey. II. Results of precursor observations.
o	Table 2: <[GHK2005] HI JHHMMSS.s+DDMMSS> N=166.
=E=	Catalogue in electronic form as J/AJ/130/2613
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHK93]
[GHK93]	(Gomez+Hartmann+Kenyon+, 1993)= (Gomez) = (Taurus)
Write:	<<[GHK93] Group R>>
N:	6
Object:	Group of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	N=6 groups in Taurus region. Each group is associated with a dark cloud.
in source:	NAME Taurus Region
Ref:	=1993AJ....105.1927G
by	GOMEZ M. , HARTMANN L., KENYON S.J., HEWETT R.
	Astron. J., 105, 1927-1937 (1993)
	On the spatial distribution of pre-main-sequence stars in Taurus.
o	Table 4: <[GHK93] Group R> (Nos I-VI).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHL2003]
[GHL2003]	(Gibb+Hoare+Little+, 2003)
Write:	<<[GHL2003] G35.2N NN>> <<[GHL2003] G35MM2>>
N:	11+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	BIMA and VLA observations of the North region of the molecular cloud G35.2-0.7. N=11 radio emission sources are observed. N=1 mm sources is found, designated as in a private communication of J.M. Carpenter. See [DLW84], [HL88].
in source:	GAL 035.2-00.74
Ref:	=2003MNRAS.339.1011G
by	GIBB A.G. , HOARE M.G., LITTLE L.T., WRIGHT M.C.H.
	Mon. Not. R. Astron. Soc., 339, 1011-1024 (2003)
	A detailed study of G35.2-0.7N: collimated outflows in a cluster of high-mass young stellar objects.
o	Table 1: <[GHL2003] G35.2N NN> (Nos 1-11). Figs 1, 6: <[GHL2003] G35MM2> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHL2013]
[GHL2013]	(Gomez-Ruiz+Hirano+Leurini+, 2013) (Not yet in Simbad)
Write:	<<[GHL2013] BNa>>
N:	7
Object:	Clump (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	SMA 1.4mm observations of the blue lobe of the LDN 1157 outflow. See also [TB95].
in source:	LDN 1157: [DE95] LDN 1157 B1 = [DE95] LDN 1157 B1
Ref:	=2013A&A...558A..94G
by	GOMEZ-RUIZ A.I. , HIRANO N., LEURINI S., LIU S.-Y.
	Astron. Astrophys., 558A, 94-94 (2013)
	The L1157 protostellar outflow imaged with the submillimeter array.
o	Fig. 6, Table 3: <[GHL2013] BNa> (Nos B0f-B0j, B1g-B1h).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHM2003]
[GHM2003]	(Gioia+Henry+Mullis+, 2003)= (NEP)
Write:	<<[GHM2003] NNNN>> <<[GHM2003] JHHMMSS.s+DDMMSS>> <<[GHM2003] RX JHHMM.m+DDMM A>> <<[GHM2003] RX JHHMM.m+DDMM AN>> <<[GHM2003] RX JHHMM.m+DDMM cfh N>>
N:	446+30
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	ROSAT All Sky Survey around North Ecliptic Pole is used to search optical identification of 446 X-ray sources. UH, CFHT and MMT observations. In the field of these 'RX JHHMM.m+DDMM' sources, other objects are found.
Ref:	=2003ApJS..149...29G
by	GIOIA I.M. , HENRY J.P., MULLIS C.R., BOHRINGER H., BRIEL U.G., VOGES W., HUCHRA J.P.
	Astrophys. J., Suppl. Ser., 149, 29-51 (2003)
	The ROSAT north ecliptic pole survey: the optical identifications.
o	Table 3, col(2): <[GHM2003] NNNN> N=446 among (Nos 1239-6570). Paragr. 6: <[GHM2003] JHHMMSS.s+DDMMSS> N=17, <[GHM2003] JHHMMSS.s+DDMMSS> = <[GHM2003] RX JHHMM.m+DDMM A> N=8, <[GHM2003] RX JHHMM.m+DDMM AN> N=3, <[GHM2003] RX JHHMM.m+DDMM cfh N> N=2.
=E=	Catalogue in electronic form as J/ApJS/149/29
=E=	Catalogue in electronic form as J/ApJS/162/304
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHM2007]
[GHM2007]	(Garcia-Barreto+Hernandez-Toledo+Moreno-Diaz+, 2007)
Write:	<<[GHM2007] NN>>
N:	90
Object:	Part of G + * + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	UBVRI photometry of NGC 3367 at the 84cm optical telescope at the Observatorio Astronomic Nacional, Mexico.
in source:	NGC 3367
Ref:	=2007AJ....134..142G
by	GARCIA-BARRETO J.A. , HERNANDEZ-TOLEDO H., MORENO-DIAZ E., BERNAL-MARIN T., VILLARREAL-CASTILLO A.L.
	Astron. J., 134, 142-157 (2007)
	UBVRI photometry of stellar structures throughout the disk of the barred galaxy NGC 3367.
o	Table 3: <Cl* NGC 2682 GHM N> (Nos 1-9). Tables 5, 6: <[GHM2007] NN> (Nos 1-90).
=E=	Catalogue in electronic form as J/AJ/134/142
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHM84]
[GHM84]	(Gallagher+Hunter+Mould, 1984)
Write:	<<[GHM84] SNR>>
N:	1
Object:	SNR (SIMBAD class: SNRemnant = SuperNova Remnant)
Stat:	is completely incorporated in Simbad
Note:	KPNO 4m Mayall telescope observations of of N=1 supernova remant candidate.
in source:	NGC 185
Ref:	=1984ApJ...281L..63G
by	GALLAGHER III J.S. , HUNTER D.A., MOULD J.
	Astrophys. J., 281, 63-65 (1984)
	A probable supernova remnant in the dwarf elliptical galaxy NGC 185.
o	<[GHM84] SNR> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHM99]
[GHM99]	(Gioia+Henry+Mullis+, 1999)
Write:	<<[GHM99] NN>>
N:	37
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	ASCA, ROSAT HRI, and Keck LRIS observations of RX J1716.6+6708 ClG. N=37 galaxies, map in Fig.1.
in source:	RX J1716.0+6708
Ref:	=1999AJ....117.2608G
by	GIOIA I.M. , HENRY J.P., MULLIS C.R., EBELING H., WOLTER A.
	Astron. J., 117, 2608-2616 (1999)
	RX J1716.6+6708: a young cluster at z=0.81.
o	Table 1: <[GHM99] NN> (Nos 1-37).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHN2008]
[GHN2008]	(Goldsmith Heyer+Narayanan+, 2008)
Write:	<<[GHN2008] N>>
N:	3
Object:	Cometary Globule (SIMBAD class: ComGlob = Cometary Globule / Pillar)
Stat:	is completely incorporated in Simbad
Note:	FCRAO 13.7m millimeter telescope observations of the Taurus molecular cloud. N=3 cometary globules are found in a large cavity.
in source:	TMC:NAME B213-B18 Cavity
Ref:	=2008ApJ...680..428G
by	GOLDSMITH P.F. , HEYER M., NARAYANAN G., SNELL R., LI D., BRUNT C.
	Astrophys. J., 680, 428-445 (2008)
	Large-scale structure of the molecular gas in Taurus revealed by high linear dynamic range spectral line mapping.
o	Table 6: <[GHN2008] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GHO
GHO	(Gunn+Hoessel+Oke)= [GHO86]
Write:	<<GHO HHMMSS+DDMMSS>>
N:	418
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Ref:	=1986ApJ...306...30G
by	GUNN J.E. , HOESSEL J.G., OKE J.B.
	Astrophys. J., 306, 30-37 (1986)
	A systematic survey for distant galaxy clusters.
o	<GHO HHMMSS+DDMMSS> N=418
=E=	Catalogue in electronic form as <J/ApJ/306/30/>
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GHO86]
[GHO86]	(Gunn+Hoessel+Oke, 1986)
*****	Avoid the usage of [GHO86], prefer GHO
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHP99]
[GHP99]	(Goetz+Howard+Pipher+, 1999) (Not yet in Simbad)
Write:	<<[GHP99] NN>>
N:	35
Object:	* (SIMBAD class: Star)
Note:	Stars in Sh 2-88B region. Paper published in American Astronomical Society Meeting 193, 7103: Extinction associated with the ultracompact HII region, S88B. Also found at http adress of first author in 2000A&A...360.1107D (Table 2 and references).
in source:	SH 2-88 B
Auth.:	GOETZ J.+
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHR2007]
[GHR2007]	(Gullieuszik+Held+Rizzi+, 2007)
Write:	<<[GHR2007] Shallow NNNNN>> <<[GHR2007] Deep NNNN>>
N:	11377+1894
Object:	(Near IR) (SIMBAD class: Star)
Note:	NTT SOFI NIR photometry of two fields (Shallow and Deep fields) in the Fornax Dwarf Galaxy.
in source:	NAME Fornax Dwarf Galaxy
Ref:	=2007A&A...467.1025G
by	GULLIEUSZIK M. , HELD E.V., RIZZI L., SAVIANE I., MOMANY Y., ORTOLANI S.
	Astron. Astrophys., 467, 1025-1036 (2007)
	Near-infrared observations of the Fornax dwarf galaxy. I. The red giant branch.
o	Table 2: <[GHR2007] Shallow NNNNN> (Nos 1-11377). Table 3: <[GHR2007] Deep NNNN> (Nos 1-1894).
=E=	Catalogue in electronic form as J/A+A/467/1025
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHR2008]
[GHR2008]	(Gullieuszik+Held+Rizzi+, 2008)
Write:	<<[GHR2008] NNNN>>
N:	2069
Object:	* (SIMBAD class: Star)
Note:	UKIRT WFCAM observations of Leo II.
in source:	Leo II = UGC 6253
Ref:	=2008MNRAS.388.1185G
by	GULLIEUSZIK M. , HELD E.V., RIZZI L., GIRARDI L., MARIGO P., MOMANY Y.
	Mon. Not. R. Astron. Soc., 388, 1185-1197 (2008)
	The evolved stars of LeoII dSph galaxy from near-infrared UKIRT/WFCAM observations.
o	Table 2: <[GHR2008] NNNN> (Nos 1-2069).
=E=	Catalogue in electronic form as J/MNRAS/388/1185
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHR99]
[GHR99]	(Girart+Ho+Rudolph+, 1999) (Not yet in Simbad)
Write:	<<[GHR99] BN>> <<[GHR99] RN>>
N:	4
Object:	Clump (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	(Nos B1-B2) blueshifted clumps (Nos R1-R2) redshifted clumps
in source:	NGC 2071
Ref:	=1999ApJ...522..921G
by	GIRART J.M. , HO P.T.P., RUDOLPH A.L., ESTALELLA R., WILNER D.J., CHERNIN L.M.
	Astrophys. J., 522, 921-934 (1999)
	The HCO^+ molecular outflow in NGC 2071.
o	p. 922 : Calibrator PK 0420 = PKS 0420-015 ?
o	Fig.8: <[GHR99] AN> (Nos B1-B2, R1-R2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHS2009]
[GHS2009]	(Gullieuszik+Held+Saviane+, 2009)
Write:	<<[GHS2009] NNN>>
N:	57
Object:	Red Giant * + * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 spectroscopy of red giant stars in the dwarf spheroidal galaxy Leo I.
in source:	UGC 5470 = Leo I
Ref:	=2009A&A...500..735G
by	GULLIEUSZIK M. , HELD E.V., SAVIANE I., RIZZI L.
	Astron. Astrophys., 500, 735-747 (2009)
	New constraints on the chemical evolution of the dwarf spheroidal galaxy Leo I from VLT spectroscopy.
o	Table 1: <[GHS2009] NNN> (Nos 1-54, 101-103).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHS99]
[GHS99]	(Gibson+Hughes+Stetson+, 1999)
Write:	<<[GHS99] RNN>> <<[GHS99] CNN>>
N:	45+20
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	HST key project on extragalactic distance scale. N=45 reference stars (Nos R1-R45) and N=20 Cepheids (Nos C1-C20), in NGC 4725. Finding charts for Cepheids figs 2, 3. See also: [FHM94], [HST94], [KIF96], [FFH96], [SHM96], [GPF97], [RMM97], [FBK98], [HHH98], [PSF98], [TFS98], [KIS99], [SHF99], [GFF99], [MHS99], [SFK99], [PKB99], [GSF2000], [MHS2000]
in source:	NGC 4725
Ref:	=1999ApJ...512...48G
by	GIBSON B.K. , HUGHES S.M.G., STETSON P.B., FREEDMAN W.L., KENNICUTT R.C.Jr, MOULD J.R., BRESOLIN F., FERRARESE L., FORD H.C., GRAHAM J.A., HAN M., HARDING P., HOESSEL J.G., HUCHRA J.P., ILLINGWORTH G.D., KELSON D.D., MACRI L.M., MADORE B.F., PHELPS R.L., PROSSER C.F., SAHA A., SAKAI S., SEBO K.M., SILBERMANN N.A., TURNER A.M.
	Astrophys. J., 512, 48-64 (1999)
	The Hubble Space Telescope key project on the extragalactic distance scale. XVII. The Cepheid distance to NGC 4725.
o	Table 2: <[GHS99] RNN> (Nos R1-R45). Table 4: <[GHS99] CNN> (Nos C1-C20).
=E=	Catalogue in electronic form as J/ApJ/512/48
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHV2000]
[GHV2000]	(Greiner+Hartmann +Voges+, 2000) (Not yet in Simbad)
Write:	<<[GHV2000] Star A>>
N:	2
Object:	* (SIMBAD class: Star)
Note:	N=2 stars (Nos A-B) in the error-box of 1RXS J061909.0+083859.
Ref:	=2000A&A...353..998G
by	GREINER J. , HARTMANN D.H., VOGES W., BOLLER T., SCHWARZ R., ZHARIKOV S.V.
	Astron. Astrophys., 353, 998-1008 (2000)
	Search for GRB X-ray afterglows in the ROSAT all-sky survey.
o	Fig.5: <[GHV2000] Star A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GHV2009]
[GHV2009]	(Garcia+Herrero+Vicente+, 2009)
Write:	<<[GHV2009] Assoc NNN>> <<[GHV2009] Star NNNNN>>
N:	198 + 32
Object:	OB Assoc. + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	INT WFC observations of IC 1613.
in source:	IC 1613
Ref:	=2009A&A...502.1015G
by	GARCIA M. , HERRERO A., VICENTE B., CASTRO N., CORRAL L.J., ROSENBERG A., MONELLI M.
	Astron. Astrophys., 502, 1015-1041 (2009)
	The young stellar population of IC 1613. I. A new catalogue of OB associations.
o	Table A.1: <[GHV2009] Assoc NNN> (Nos 1-198). Table 5, Table A.2: <[GHV2009] Star NNNNN> N=32 among (Nos 1703-83197).
Ref:	=2010A&A...523A..23G
by	GARCIA M. , HERRERO A., CASTRO N., CORRAL L., ROSENBERG A.
	Astron. Astrophys., 523A, 23-23 (2010)
	The young stellar population of IC 1613. II. Physical properties of OB associations.
o	Table 1: <[GHC2010b] NNN> N=166 among (Nos 2-197). Table 4: <[GHV2009] Star NNNN> N=13 among (Nos 52443-75661).
=E=	Catalogue in electronic form as J/A+A/502/1015
=E=	Catalogue in electronic form as <J/A+A/523/A23/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GHVC
GHVC	(GASS High Velocity Cloud)
Write:	<<GHVC GLLL.l+BB.b+VVV>>
N:	about 2000
Object:	HVC (SIMBAD class: HVCld = High-velocity Cloud)
Note:	We are publishing a catalogue of high velocity clouds as discovered within the Galactic All Sky Survey (GASS) data. The catalogue paper is nearing submission and will contain a table of all HVCs found in GASS. We are submitting this application for a new acronym in order to facilitate reference to specific GASS HVCs in future follow-up work. The sensitivity of GASS to large scale structure as well as the way we identify HVCs using a floodfill sourcefinder makes a GHVC distinct from an HVC, in that our definition of a source may join several clouds that are connected at the 2 sigma level. Hence, we propose the new acronym GHVC to specifically designate a source as a GASS HVC, to make the origin of such a cloud clear.
Ref:	=2013ApJS..209...12M
by	MOSS V.A. , McCLURE-GRIFFITHS N.M., MURPHY T., PISANO D.J., KUMMERFELD J.K., CURRAN J.R.
	Astrophys. J., Suppl. Ser., 209, 12 (2013)
	High-velocity clouds in the Galactic All Sky Survey. I. Catalog.
o	Table 1: <GHVC GLLL.l+BB.b+VVV> N=1693. Table 2: <GAVC GLLL.l+BB.b+VVV> N=295. University of Sydney/CSIRO Astronomy and Space Science
=E=	Catalogue in electronic form as J/ApJS/209/12
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [GIB2004]
[GIB2004]	(Greve+Ivison+Bertoldi+, 2004)= (LH) = MAMBO
Write:	<<[GIB2004] MM JHHMMSS+DDMM>> <<[GIB2004] N2 1200.NN>> <<[GIB2004] LE 1200.NNN>> <<[GIB2004] LH 1200.NNN>> (not recognised by Simbad, but found in literature)
N:	21+23+5
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	Max-Planck Millimeter Bolometer survey (MAMBO) of the Lockman Hole and ELAIS N2 fields at 1200 mu.m. See also [IGS2004].
in source:	NAME Lockman Hole
in source:	ELAIS N2
Ref:	=2004MNRAS.354..779G
by	GREVE T.R. , IVISON R.J., BERTOLDI F., STEVENS J.A., DUNLOP J.S., LUTZ D., CARILLI C.L.
	Mon. Not. R. Astron. Soc., 354, 779-797 (2004)
	A 1200-µm MAMBO survey of ELAISN2 and the Lockman Hole - I. Maps, sources and number counts.
o	Table 1: <[GIB2004] MM JHHMMSS+DDMM> N=21 = <[GIB2004] N2 1200.NN> (Nos 1-21). Table 2: <[GIB2004] MM JHHMMSS+DDMM> N=23 = <[GIB2004] LE 1200.NN> (Nos 1-23).
Ref:	=2005MNRAS.364.1025I
by	IVISON R.J. , SMAIL I., DUNLOP J.S., GREVE T.R., SWINBANK A.M., STEVENS J.A., MORTIER A.M.J., SERJEANT S., TARGETT T.A., BERTOLDI F., BLAIN A.W., CHAPMAN S.C.
	Mon. Not. R. Astron. Soc., 364, 1025-1040 (2005)
	A robust sample of submillimetre galaxies: constraints on the prevalence of dusty, high-redshift starbursts.
o	Table 1, notes: <[GIB2004] LE 1200.NNN> (Nos 42, 96, 104, 182, 213) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GIB2011]
[GIB2011]	(Ghandi+Isobe+Birkenshaw+, 2011)
Write:	<<[GIB2011] NN>>
N:	22
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Subaru COMICS mid-IR observations of M82.
in source:	M 82 = NGC 3034
Ref:	=2011PASJ...63S.505G
by	GHANDI P. , ISOBE N., BIRKINSHAW M., WORRALL D.M., SALKON I., IWASAWA K., BAMBA A.
	PASJ, 63S, 505-521 (2011)
	Diffraction-limited Subaru imaging of M82: Sharp mid-infrared view of the starburst core.
o	Table 1: <[GIB2011] NN> (Nos 1-22).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GIBS
GIBS	(GIRAFFE Inner Bulge Survey)
Write:	<<GIBS NNNN>>
N:	6392
Object:	Red Clump * (SIMBAD class: Star)
Note:	VLT FLAMES observations of N=6392 red clump stars, as part of the Giraffe Inner Bulge Survey (GIBS). See also the webpage of the GIBS team: http://milkywaybulgelp.wordpress.com/
Ref:	=2014A&A...562A..66Z
by	ZOCCALI M. , GONZALEZ O.A., VASQUEZ S., HILL V., REJKUBA M., VALENTI E., RENZINI A., ROJAS-ARRIAGADA A., MARTINEZ-VALPUESTA I., BABUSIAUX C., BROWN T., MINNITI D., McWILLIAM A.
	Astron. Astrophys., 562A, 66-66 (2014)
	The GIRAFFE Inner Bulge Survey (GIBS). I. Survey description and a kinematical map of the Milky Way bulge.
o	Table 2: <GIBS NNNN> (Nos 1-6392).
=E=	Catalogue in electronic form as J/A+A/562/A66
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Giclas
Giclas	(Giclas)
====>	Equivalent to: G
Details on Acronym: [GIL2005]
[GIL2005]	(Green+Infante+Lopez+, 2005)
Write:	<<[GIL2005] Cluster>> <<[GIL2005] NN>> <<[GIL2005] g>>
N:	1+21+1
Object:	Cluster of G + G (SIMBAD class: Galaxy)
Note:	VLT FORS2 observations of the field around UM 425. Confirmation of a cluster of galaxies (see also [MW2003]). Near UM 245B a faint galaxy 'g' is observed.
Ref:	=2005ApJ...630..142G
by	GREEN P.J. , INFANTE L., LOPEZ S., ALDCROFT T.L., WINN J.N.
	Astrophys. J., 630, 142-151 (2005)
	Discovery of a galaxy cluster in the foreground of the wide-separation quasar pair UM 425.
o	Text: <[GIL2005] Cluster> N=1. Table 1: <[GIL2005] NN> N=21 among (Nos 2-39). Text: <[GIL2005] g> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Gilmore
Gilmore	(Gilmore)= (22h) = (F117) = (F867)
Write:	<<Gilmore 22h NNN>> <<Gilmore 22h NN-NN>> <<Gilmore F117 NN-NN>> <<Gilmore F867 NNN>> <<Gilmore F867 NN-NN>>
Object:	* (SIMBAD class: Star)
Note:	3 catalogues provided by Gilmore: The 22h, F117 and F867 catalogues are cited in 1989MNRAS.238..225S. The 22h catalogue is described in 1985MNRAS.213..257G.
Auth.:	GILMORE G.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GIN
GIN	(Galaxy Id. Number)
Write:	<<GIN NNN>>
N:	795
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table 3: N=743 program galaxies (Nos 1-742) and No. 901, and N=52 calibration galaxies (Nos 750-801) all GIN are cross-id. with [WCB96] in col.(2). See also the ClG numbering CID NN in Table 1, and ClG numbering CAN in Paper II.
Ref:	=1996ApJS..106....1W
by	WEGNER G. , COLLESS M., BAGGLEY G., DAVIES R.L., BERTSCHINGER E., BURSTEIN D., McMAHAN R.K.Jr, SAGLIA R.P.
	Astrophys. J., Suppl. Ser., 106, 1-26 (1996)
	The peculiar motions of early-type galaxies in two distant regions. I. Cluster and galaxy selection.
o	Table 1: <CID NN> (Nos 1-84, 90), with N=49 cross-id. in last col.: <[WCB96] ACO NNN-N>, <[WCB96] ACO NNNN-W>, <[WCB96] JNN>, <[WCB96] JNN-N>, <[WCB96] JNNW>, <[WCB96] PNNN-N>. Table 3: <GIN NNN> (Nos 1-801), with N=749 cross-id. in col.(2): <[WCB96] ACO NNNN A>, <[WCB96] ACO NNNN N>, <[WCB96] ACO NNN-N A>, <[WCB96] ACO NNN-N N>, <[WCB96] ACO NNNN-W A>, <[WCB96] ACO NNNN-W N>, <[WCB96] JNN A>, <[WCB96] JNN N>, <[WCB96] JNN/NN N>, <[WCB96] JNN-N A>, <[WCB96] JNN-N N>, <[WCB96] JNNW A>, <[WCB96] JNNW N>, <[WCB96] PNNN-N A>, <[WCB96] PNNN-N N>
=E=	Catalogue in electronic form as J/ApJS/106/1
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Ginga
Ginga	(Ginga satellite)= (GS)
Write:	<<Ginga HHMM+DD>> <<Ginga HHMM+DDd>> <<Ginga HHMM.m+DDMM>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	1st reference from this satellite (usually found as GS in the literature). In this ref., N=1 (X) source.
Ref:	=1990ApJ...356L..47K
by	KOYAMA K. , KAWADA M., TAKEUCHI Y., TAWARA Y., USHIMARU N., DOTANI T., TAKIZAWA M.
	Astrophys. J., 356, 47-50 (1990)
	Discovery of a peculiar X-ray pulsar GS 1843+00.
o	First ref. from this satellite. In this ref. <Ginga HHMM+DD> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Giovanelli
Giovanelli	(Giovanelli)
Write:	<<Giovanelli NNN>>
N:	799
Object:	HVC, IVC (SIMBAD class: Cloud)
Ref:	=1980AJ.....85.1155G
by	GIOVANELLI R.
	Astron. J., 85, 1155-1181 (1980)
	Studies of high-velocity clouds. I. A high-sensitivity survey.
o	Table II: <Giovanelli NNN> (Nos 1-799)
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [GIP2003]
[GIP2003]	(Greve+Ivison+Papadopoulos, 2003)
Write:	<<[GIP2003] J164502-SMM1>>
N:	1
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	A 850mu.m SCUBA map of ERO [DGI99] J164502+4626.4 shows that it contains at least two sources: one coincident with the ERO and a second designated by the authors as 'J164502-SMM1'.
Ref:	=2003ApJ...599..839G
by	GREVE T.R. , IVISON R.J., PAPADOPOULOS P.P.
	Astrophys. J., 599, 839-846 (2003)
	Gas and dust in the extremely red object ERO J164502+4626.4.
o	Table 2: <[GIP2003] J164502-SMM1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GIP2004]
[GIP2004]	(Greve+Ivison+Papadopoulos, 2004) (Not yet in Simbad)
Write:	<<[GIP2004] 4C 60.07 A>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA maps of 4C 60.07: N=3 radio hot spots A to C.
Ref:	=2004A&A...419...99G
by	GREVE T.R. , IVISON R.J., PAPADOPOULOS P.P.
	Astron. Astrophys., 419, 99-107 (2004)
	Detection of CO J = 1-0 in the z = 3.79 radio galaxy 4C60.07.
o	Fig.1: <[GIP2004] 4C 60.07 A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GIP2007]
[GIP2007]	(Guseva+Izotov+Papaderos+, 2007) (Not yet in Simbad)
Write:	<<[GIP2007] HS 2236+1344a>> <<[GIP2007] UM NNNa>> <<[GIP2007] Mrk 1236a>> <<[GIP2007] cgcg007-025a>> <<[GIP2007] Tol 65a>> <<[GIP2007] J02481595-08171651a>> <<[GIP2007] Pox NNNa>> <<[GIP2007] IC 4662a>>
N:	29
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	HII in 10 galaxies.
in source:	HS 2236+1344
in source:	UM 461
in source:	UM 462
in source:	Z 7-25
in source:	Tol 65
in source:	SDSS J024815.0-081716.0
in source:	POX 4
in source:	POX 120
in source:	IC 4662
Ref:	=2007A&A...464..885G
by	GUSEVA N.G. , IZOTOV Y.I., PAPADEROS P., FRICKE K.J.
	Astron. Astrophys., 464, 885-893 (2007)
	Balmer jump temperature determination in a large sample of low-metallicity HII regions.
o	Table 3: <[GIP2007] HS 2236+1344a> (Nos a-b), <[GIP2007] UM 461a> (Nos a-b), <[GIP2007] UM 462a> (Nos a-b), <[GIP2007] Mrk 1236a> (Nos a-c), <[GIP2007] cgcg007-025a> (Nos a-d), <[GIP2007] Tol 65a> (Nos a-b), <[GIP2007] J02481595-08171651a> (Nos a-b), <[GIP2007] Pox 4a> (Nos a-b), <[GIP2007] Pox 120a> (Nos a-b), <[GIP2007] IC 4662a> (Nos a-e).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GIR89]
[GIR89]	(Ghosh+Iyengar+Rengarajan+, 1989)
Write:	<<[GIR89] W31 SNN>> <<[GIR89] G10.2-0.3 NN>> <<[GIR89] G10.3-0.1 N>>
N:	12+26+5
Object:	(IR) + (Rad) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	TIFR balloon borne experiment. Table 1: N=12 150mu.m sources, map Figs 1-4. Table 2: N=26 radio-sources in the HII region Gal 10.2-0.3. Table 3: N=5 radio-sources in the HII region Gal 10.3-0.1.
in source:	W 31
Ref:	=1989ApJ...347..338G
by	GHOSH S.K. , IYENGAR K.V.K., RENGARAJAN T.N., TANDON S.N., VERMA R.P., DANIEL R.R., HO P.T.P.
	Astrophys. J., 347, 338-348 (1989)
	Far-infrared and radio observations of ther W 31 star-forming region.
o	Table 1: <[GIR89] W31 SNN> (Nos S1-S12). Table 2: <[GIR89] G10.2-0.3 NN> (Nos 1-26). Table 3: <[GIR89] G10.3-0.1 N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GIRL
GIRL	(Galactic IR Loop)
Write:	<<GIRL GLLL+BB>>
N:	156+317
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	First cited in Kauff H.U., Siebenmorgen R. (eds.), 1996, ESO workshop, Springer, p.125: The role of dust in the formations of star. Catalogue of IRAS loops in the 4 galactic quadrants.
Ref:	=2004A&A...418..131K
by	KISS C. , MOOR A., TOTH L.V.
	Astron. Astrophys., 418, 131-141 (2004)
	Far-infrared loops in the 2nd Galactic Quadrant.
o	About 150 associated objects not identified.
o	tablea: <GIRL GLLL+BB> N=145.
Ref:	=2007A&A...463.1227K
by	KOENYVES V. , KISS C., MOOR A., KISS Z.T., TOTH L.V.
	Astron. Astrophys., 463, 1227-1234 (2007)
	Catalogue of far-infrared loops in the Galaxy.
o	Appenb: <GIRL GLLL+BB> N=317.
=E=	Catalogue in electronic form as J/A+A/418/131
=E=	Catalogue in electronic form as J/A+A/463/1227
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: GISMO
GISMO	(Goddard IRAM Superconducting Millimeter Observer) (Not yet in Simbad)
*****	Avoid the usage of GISMO, prefer [MKS2019]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GIU
GIU	(Giuffrida et al, 2009, Sgr dSph wide angle photometry)
Write:	<<GIU JHHMMSSss+DDMMSSss>> <<GIU JHHMMSS.ss+DDMMSS.s>>
N:	270683
Object:	* (SIMBAD class: Star)
Note:	VLT VIMOS observations across the major and minor axis of Sgr dSph.
Ref:	=2010A&A...513A..62G
by	GIUFFRIDA G. , SBORDONE L., ZAGGIA S., MARCONI G., BONIFACIO P., IZZO C., SZEIFERT T., BUONANNO R.
	Astron. Astrophys., 513A, 62-62 (2010)
	A wide angle view of the Sagittarius dwarf spheroidal galaxy. I. VIMOS photometry and radial velocities across Sgr dSph major and minor axis.
o	Table catalog : all stars with a velocity measurement have been ingested in SIMBAD (812 objects); many coordinates are shifted by 2 to 3''.
o	<GIU JHHMMSS.ss+DDMMSS.s> N=270683. Max-Planck Institute for Astrophysiscs, Garching, Germany
=E=	Catalogue in electronic form as J/A+A/513/A62
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: GJ
GJ	(Gliese+Jahreiss)= Gl = Gls = Gliese = (NN) = (NSC)
Write:	<<GJ NNNNA>> <<GJ NNNNa>> <<GJ NNN.NA>> <<GJ NNN.Na>>
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	1991: Preliminary Version of the Third Catalogue of Nearby Stars (Catalogue V/70), found has CNS3. Stars labelled 'NN', without format, have been numbered (Nos 3001-4388).
Ref:	=1969VeARI..22....1G
by	GLIESE W.
	Veroeff. Astron. Rechen-Inst. Heidelberg, 22, 1-None (1969)
	Catalogue of nearby stars.
o	<GJ NNN.NA> (Nos 1.0-965.0), N=1529
Ref:	=1979A&AS...38..423G
by	GLIESE W. , JAHREISS H.
	Astron. Astrophys., Suppl. Ser., 38, 423-448 (1979)
	Nearby star data published 1969-1978.
o	Table 1: <GJ NNNN> (Nos 1000-1294). Table 2: <GJ NNNN> (Nos 2001-2159)
=E=	Catalogue in electronic form as V/35
=E=	Catalogue in electronic form as V/70
Details on Acronym: GJ
GJ	(Gliese+Jahreiss)= Gl = Gliese = (W) = (WEPP) = (Wo) = (Woolley)
Write:	<<GJ 9NNNA>> <<GJ 9NNNa>>
N:	848
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Extension of the Gliese catalogue , by Woolley+ The authors have assigned to the newly added stars numbers starting at 9001 in order of 1950 right ascension. Tables Ia and Ib: (Nos 9001-9850) No. 9419 subsequently removed since new parallax measurement while Nos 9849 and 9840 were added. The tables also contain other Gliese stars (GJ). No Identif. charts.
Ref:	=1970ROAn....5....1W
by	WOOLLEY R. , EPPS E.A., PENSTON M.J., POCOCK S.B.
	R. Obs. Ann., 5, 1-None (1970)
	Catalogue of stars within 25 parsecs of the Sun.
o	<GJ NNNN> (Nos 9001-9850)
=E=	Catalogue in electronic form as V/32
Details on Acronym: [GJE2020]
[GJE2020]	(Guo+Jiang+Egami+, 2020)
Write:	<<[GJE2020] NNN>>
N:	166
Object:	LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	MMT Hectospec and Magellan M2FS spectroscopy of N=166 Lymanα emitters (LAEs). Use of archival Subaru Suprime-Cam data.
in source:	NAME SXDF
Ref:	=2020ApJ...902..137G
by	GUO Y. , JIANG L., EGAMI E., NING Y., ZHENG Z.-Y., HO L.C.
	Astrophys. J., 902, 137-137 (2020)
	A spectroscopic survey of Lyα emitters at z ≃ 3.1 over ~1.2 °^{2}.
o	Table 2: <[GJE2020] NNN> (Nos 1-166).
=E=	Catalogue in electronic form as <J/ApJ/902/137/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GJG2017]
[GJG2017]	(Gordon+Jones+Gehrz+, 2017)
Write:	<<[GJG2017] N159A A>> <<[GJG2017] N159 Papillon A>> <<[GJG2017] N160 A>>
N:	14
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	SOFIA FORCAST and Spitzer IRAC observations of N=14 infrared sources in N159A, N159 Papillon, and N160, three star-forming HII regions of the LMC. Use of archival Herschel PACS 100µm data. Use of 2MASS data.
in source:	Magellanic Clouds:LMC:LHA 120-N 159A = LHA 120-N 159A
in source:	Magellanic Clouds:LMC:Papillon Nebula in the LMC = Papillon Nebula in the LMC
in source:	Magellanic Clouds:LMC:LHA 120-N 160 = LHA 120-N 160
Ref:	=2017ApJ...834..122G
by	GORDON M.S. , JONES T.J., GEHRZ R.D., HELTON L.A.
	Astrophys. J., 834, 122-122 (2017)
	Massive star formation in the LMC. I. N159 and N160 complexes.
o	Fig. 3, Table 2: <[GJG2017] N159A A> (Nos A-E). Fig. 4, Table 2: <[GJG2017] N159 Papillon A> (Nos A-C). Fig. 5, Table 2: <[GJG2017] N160 A> (Nos A-F).
=E=	Catalogue in electronic form as <J/ApJ/834/122/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GJH92]
[GJH92]	(Gomez+Jones+Hartmann+, 1992)= (J2-)
Write:	<<[GJH92] NNNN>>
N:	3 among 2041
Object:	PMS* (SIMBAD class: YSO = Young Stellar Object)
Note:	These stars are found in the literature as 'J2'. N=3, Nos 157, 642, 2041. The corresponding 'J1' designation is [HJS91] in SIMBAD.
Ref:	=1992AJ....104..762G
by	GOMEZ M. , JONES B.F., HARTMANN L., KENYON S.J., STAUFFER J.R., HEWETT R.
	Astron. J., 104, 762-773 (1992)
	On the ages of pre-main-sequence stars in Taurus.
o	J2-NNNN: use <[GJH92] NNNN> N=3 (Nos 157, 642, 2041)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GJJC
GJJC	(Gillett+Jacoby+Joyce+Cohen+)
Write:	<<PN GJJC N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	GJJC 1 = PN G009.8-07.5
Ref:	=1989ApJ...338..862G
by	GILLETT F.C. , JACOBY G.H., JOYCE R.R., COHEN J.G., NEUGEBAUER G., SOIFER B.T., NAKAJIMA T., MATTHEWS K.
	Astrophys. J., 338, 862-874 (1989)
	The optical/infrared counterpart(s) of IRAS 18333-2357.
o	<PN GJJC N> (No. 1).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GJL92]
[GJL92]	(Goodman+Jones+Lada+, 1992)
Write:	<<[GJL92] HHMMSS.s+DDMMSS>>
N:	22
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=18 stars + 2 embedde obj. + 2 unpolarized sources
in source:	NAME Barn 216-217 Dark Cloud
Ref:	=1992ApJ...399..108G
by	GOODMAN A.A. , JONES T.J., LADA E.A., MYERS P.C.
	Astrophys. J., 399, 108-113 (1992)
	The structure of magnetic fields in dark clouds : infrared polarimetry in B 216-217.
o	<NAME BARN 216-217 DARK CLOUD>. Table 1: <[GJL92] HHMMSS.s+DDMMSS> N=22
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GJL95]
[GJL95]	(Goodman+Jones+Lada+, 1995)
Write:	<<[GJL95] NN>>
N:	53
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	LDN 1755
Ref:	=1995ApJ...448..748G
by	GOODMAN A.A. , JONES T.J., LADA E.A., MYERS P.C.
	Astrophys. J., 448, 748-765 (1995)
	Does near-infrared polarimetry reveal the magnetic field in cold dark clouds?
o	Table 1: <[GJL95] NN> (Nos 1-53)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GJL99]
[GJL99]	(Guirado+Jones+Lara+, 1999) (Not yet in Simbad)
Write:	<<[GJL99] WWXN>> <<[GJL99] WWSN>>
N:	7+4
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Components structures of [SNP90] 1830-211 NE and SW. At 8.4GHz (NEX1-NEX5) and (SWX1-SWX2). At 2.4GHz (NES1-NES3) and (SWS1).
in source:	PKS 1830-211
in source:	[SNR90] 1830-211 NE
in source:	[SNR90] 1830-211 SW
Ref:	=1999A&A...346..392G
by	GUIRADO J.C. , JONES D.L., LARA L., MARCAIDE J.M., PRESTON R.A., RAO A.P., SHERWOOD W.A.
	Astron. Astrophys., 346, 392-396 (1999)
	Dual-frequency VLBI observations of the gravitational lens system PKS 1830-211.
o	Fig.1: <[GJL99] WWXN> (Nos NEX1-NEX5, SWX1-SWX2). Fig.2: <[GJL99] WWSN> (Nos NES1-NES3, SWS1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GJN2002]
[GJN2002]	(Garay+Johansson+Nyman+, 2002)
Write:	<<[GJN2002] A>> <<[GJN2002] N>>
N:	6+7
Object:	Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	SEST observations. N=6 clouds (Nos A-F) and N=7 clumps (Nos 1-7).
in source:	Magellanic Clouds:LMC:LMC-CO 37 = LMC-CO 37
Ref:	=2002A&A...389..977G
by	GARAY G. , JOHANSSON L.E.B., NYMAN L.-A., BOOTH R.S., ISRAEL F.P., KUTNER M.L., LEQUEUX J., RUBIO M.
	Astron. Astrophys., 389, 977-992 (2002)
	Results of the SEST Key Programme: CO in the Magellanic Clouds. VIII. The giant molecular complex No. 37 of the LMC.
o	complex No. 37 = LMC-CO 37.
o	Table 1: <[GJN2002] A> (Nos A-F), <[GJN2002] N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GJP2000]
[GJP2000]	(Garnavich+Jha+Pahre+, 2000)
Write:	<<[GJP2000] A>>
N:	5
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=5 secondary standards near GRB 991216. Finding chart in Fig.1. See also [SMP2000].
Ref:	=2000ApJ...543...61G
by	GARNAVICH P.M. , JHA S., PAHRE M.A., STANEK K.Z., KIRSHNER R.P., GARCIA M.R., SZENTGYORGYI A.H., TONRY J.L.
	Astrophys. J., 543, 61-65 (2000)
	RJK band observations of the optical afterglow of GRB 991216.
o	Table 1: <[GJP2000] A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GJP96]
[GJP96]	(Grainge+Jones+Pooley+, 1996)
Write:	<<[GJP96] N>>
N:	6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
in source:	ACO 1413
Ref:	=1996MNRAS.278L..17G
by	GRAINGE K. , JONES M., POOLEY G., SAUNDERS R., BAKER J., HAYNES T., EDGE A.
	Mon. Not. R. Astron. Soc., 278, 17-22 (1996)
	A resolved image of the Sunyaev-Zel'dovich effect in Abell 1413.
o	Table 2: <[GJP96] N> (Nos 1-6)
Details on Acronym: GJTGTZ
GJTGTZ	(Galadi-Enriquez+Jordi+Trullols+Guibert+Tian+Zhao)
Write:	<<GJTGTZ NNNNNN>>
N:	107924
Object:	* in Cl* (SIMBAD class: Star)
Note:	Paper II: N=51846 stars among (Nos 3-107924) in the open clusters NGC 1750 and 1758. See also Paper I: GJTR
in source:	NGC 1750
in source:	NGC 1758
Ref:	=1998A&AS..131..239G
by	GALADI-ENRIQUEZ D. , JORDI C., TRULLOLS E., GUIBERT J., TIAN K.P., ZHAO J.L.
	Astron. Astrophys., Suppl. Ser., 131, 239-258 (1998)
	The overlapping open clusters NGC 1750 and NGC 1758. II. (BVR) photographic photometry and proper motions.
o	Table 6: <GJTGTZ NNNNNN> N=51846 among (Nos 3-107924)
=E=	Catalogue in electronic form as J/A+AS/131/239
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GJTR
GJTR	(Galadi-Enriquez+Jordi+Trullols+Ribas)
Write:	<<GJTR NNNN>>
N:	3224
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Paper I: N=3324 stars among 3229 (5 have been eliminated, because of anomalous data), in the open clusters NGC 1750 and 1758. See also Paper II: GJTGTZ
in source:	NGC 1750
in source:	NGC 1758
Ref:	=1998A&A...333..471G
by	GALADI-ENRIQUEZ D. , JORDI C., TRULLOLS E., RIBAS I.
	Astron. Astrophys., 333, 471-478 (1998)
	The overlapping open clusters NGC 1750 and NGC 1758. I. UBVRI-CCD photometry.
o	Table 5: <GJTR NNNN> N=3324 among 3229.
=E=	Catalogue in electronic form as J/A+A/333/471
Origin	of the Acronym: L (1998A&AS..131..239G)
Details on Acronym: [GK2001]
[GK2001]	(Gomez+Kenyon, 2001)
Write:	<<[GK2001] NNN>>
N:	118
Object:	PMS* (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	New candidate PMS* in Cha I dark cloud.
in source:	NAME Cha I
Ref:	=2001AJ....121..974G
by	GOMEZ M. , KENYON S.J.
	Astron. J., 121, 974-983 (2001)
	A near-infrared imaging survey of the Chamaeleon I dark cloud.
o	Tables 3, 4: <[GK2001] NNN> (Nos 1-118).
=E=	Catalogue in electronic form as J/AJ/121/974
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GK2005]
[GK2005]	(Gutierrez+Krawczynski, 2005)
Write:	<<[GK2005] A>>
N:	6
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of the field of ACO 115.
in source:	ACO 115
Ref:	=2005ApJ...619..161G
by	GUTIERREZ K. , KRAWCZYNSKI H.
	Astrophys. J., 619, 161-168 (2005)
	The off-axis galaxy cluster merger A115.
o	Table 1: <[GK2005] A> (Nos A-F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GK2009]
[GK2009]	(Grave+Kumar, 2009) (Not yet in Simbad)
Write:	<<[GK2009] JHHMMm+DDMMmmsN>>
N:	68
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Search for infrared counterparts of high mass protostellar objects.
Ref:	=2009A&A...498..147G
by	GRAVE J.M.C. , KUMAR M.S.N.
	Astron. Astrophys., 498, 147-159 (2009)
	Spitzer-IRAC GLIMPSE of high mass protostellar objects. II. SED modelling of a bona fide sample.
o	Table 1: <[GK2009] HHMMm+DDMMmmsN> N=68.
=E=	Catalogue in electronic form as J/A+A/498/147
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GK65]
[GK65]	(Goldsmith+Kinman, 1965)
Write:	<<[GK65] 3C 345 A>>
N:	9
Object:	* (SIMBAD class: Star)
Note:	Comparison stars in the field of 3C 345. Finding chart.
Ref:	=1965ApJ...142.1693G
by	GOLDSMITH D.W. , KINMAN T.D.
	Astrophys. J., 142, 1693-1696 (1965)
	The optical variability of 3C 345.
o	Table 1: <[GK65] 3C 345 A> (Nos A-I).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKC2000]
[GKC2000]	(Garnavich+Kirshner+Challis, 2000)
Write:	<<[GKC2000] Spot N>>
N:	6
Object:	Spot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST WFPC2 observations. N=6 individual spots are developing in the ring of SN 1987A. Also designated as [LSB2000] 6 first spots.
in source:	Magellanic Clouds:LMC:SN 1987A = SN 1987A
Ref:	=2000IAUC.7360R...1G
by	GARNAVICH P. , KIRSHNER R., CHALLIS P.
	IAU Circ., 7360, 1-None (2000)
	Supernova 1987A in the Large Magellanic Cloud.
o	star projected on the ring = [WS90] 2 or 3 or 4 or 5?
o	<[GKC2000] Spot N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKC2003]
[GKC2003]	(Gustafsson+Kristensen+Clenet+, 2003)
Write:	<<[GKC2003] NNa>>
N:	23
Object:	H2 (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	GriF is used on the CFH telescope to search for H2 emitting peaks regions in OMC 1.
in source:	OMC:OMC 1 = OMC 1
Ref:	=2003A&A...411..437G
by	GUSTAFSSON M. , KRISTENSEN L.E., CLENET Y., FIELD D., LEMAIRE J.L., PINEAU DES FORETS G., ROUAN D., LE COARER E.
	Astron. Astrophys., 411, 437-446 (2003)
	New insight into shocks and star formation in Orion: First light with GriF.
o	Fig.4, Table 1: <[GKC2003] NNa> (Nos 1-19), N=23.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKD2002]
[GKD2002]	(Gouliermis+Keller+De Boer+, 2002)
Write:	<<[GKD2002] NNNN>>
N:	21
Object:	Be* (SIMBAD class: Be* = Be Star)
Note:	Siding Spring Observatory 1m telescope photometric observations of N=3 stellar association LH 91, LH 91-I and LH 95 in the LMC.
in source:	LH 95
in source:	LH 91
in source:	LMC-SGS 4
Ref:	=2002A&A...381..862G
by	GOULIERMIS D. , KELLER S.C., DE BOER K.S., KONTIZAS M., KONTIZAS E.
	Astron. Astrophys., 381, 862-883 (2002)
	Three stellar associations and their field east of LMC 4 in the Large Magellanic Cloud.
o	Table 1: <[GKD2002] NNNN> N=21 among (Nos 12-1388).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKD84]
[GKD84]	(Goss+Kalberla+Dickel, 1984)
Write:	<<[GKD84] R>> <<[GKD84] HHMMSS+DDMMSS>>
N:	16+12
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Note:	WSRT observations of N=16 H2CO clumps, and N=12 HI features probably associated with a clump in Cas A. See also [RG2002b].
in source:	NAME Cas A
Ref:	=1984A&A...139..317G
by	GOSS W.M. , KALBERLA P.M.W., DICKEL H.R.
	Astron. Astrophys., 139, 317-329 (1984)
	Westerbork observations of 6cm H2CO in the direction of Cas A.
o	Table 2: <[GKD84] R> (Nos I-XVI). Table 4: <[GKD84] HHMMSS+DDMMSS> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKE2012]
[GKE2012]	(Griffith+Kirkpatrick+Eisenhardt+, 2012)
Write:	<<[GKE2012] JHHMMSS.ss+DDMMSS.s>> <<[GKE2012] JHHMMSS.s+DDMMSS.s>>
N:	1510+906
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Spitzer 3.6 and 4.5µm photometry for N=1510 brown dwarf candidates, N=906 HyLIRG candidates, N=733373 sources in the complete photometric catalog. Use of WISE (including internal source lists) and 2MASS data.
Ref:	=2012AJ....144..148G
by	GRIFFITH R.L. , KIRKPATRICK J.D., EISENHARDT P.R.M., GELINO C.R., CUSHING M.C., BENFORD D., BLAIN A., BRIDGE C.R., COHEN M., CUTRI R.M., DONOSO E., JARRETT T.H., LONSDALE C., MACE G., MAINZER A., MARSH K., PADGETT D., PETTY S., RESSLER M.E., SKRUTSKIE M.F., STANFORD S.A., STERN D., TSAI C.-W., WRIGHT E.L., WU J., YAN L.
	Astron. J., 144, 148 (2012)
	Spitzer photometry of WISE-selected brown dwarf and hyper-luminous infrared galaxy candidates.
o	Table 1 : only spectroscopically confirmed brown dwarfs have been processed in Simbad. Tables 2 and 3 will not be ingested in Simbad.
o	Table 1: <[GKE2012] JHHMMSS.ss+DDMMSS.s> N=1510. Table 2: <[GKE2012] JHHMMSS.s+DDMMSS.s> N=906.
=E=	Catalogue in electronic form as <J/AJ/144/148/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKE2015]
[GKE2015]	(Gazak+Kudritzki+Evans+, 2015)
Write:	<<[GKE2015] NNN>>
N:	27
Object:	Red Supergiant (SIMBAD class: Star)
Note:	VLT KMOS spectroscopic observations of N=27 red supergiants (RSGs) in the Sculptor Galaxy NGC 300. Use of archival HST ACS and WFPC2 images.
in source:	NGC 300
Ref:	=2015ApJ...805..182G
by	GAZAK J.Z. , KUDRITZKI R., EVANS C., PATRICK L., DAVIES B., BERGEMANN M., PLEZ B., BRESOLIN F., BENDER R., WEGNER M., BONANOS A.Z., WILLIAMS S.J.
	Astrophys. J., 805, 182 (2015)
	Red supergiants as cosmic abundance probes: the Sculptor galaxy NGC 300.
o	Tables 2,4: <[GKE2015] NNN> N=27 among (Nos 6-140).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKE2019]
[GKE2019]	(Gilbert+Kirby+Escala+, 2019)
Write:	<<[GKE2019] NNNNNNN>>
N:	61
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Keck DEIMOS observations of N=61 stars with [Fe/H] measurements in M31's giant stellar stream. See also [EKG2019], [EGK2020], and [EKG2020].
in source:	NAME Andromeda Stream
Ref:	=2019ApJ...883..128G
by	GILBERT K.M. , KIRBY E.N., ESCALA I., WOJNO J., KALIRAI J.S., GUHATHAKURTA P.
	Astrophys. J., 883, 128-128 (2019)
	Elemental abundances in M31: first α and iron abundance measurements in M31's giant stellar stream.
o	<[GKE2019] NNNNNNN> N=61 among (Nos 2070316-2075349).
=E=	Catalogue in electronic form as <J/ApJ/883/128/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKF2005]
[GKF2005]	(Grutzbauch+Kelm+Focaldi+, 2005)
Write:	<<[GKF2005] New N>> <<[GKF2005] NNNNN>>
N:	2+15+99
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Note:	ESO 3.6m EFOSC2 observations of the NGC 4756 Group of Galaxies. Two new members among the dominant members are found, and N=15 bright + N=99 faint group member candidates.
in source:	NAME NGC 4756 GROUP
Ref:	=2005AJ....129.1832G
by	GRUETZBAUCH R. , KELM B., FOCARDI P., TRINCHIERI G., RAMPAZZO R., ZEILINGER W.W.
	Astron. J., 129, 1832-1848 (2005)
	Small-scale systems of galaxies. II. Properties of the NGC 4756 group of galaxies.
o	Fig.1, Table 3: <[GKF2005] New N> (Nos 1-2). Tables 6, 7: <[GKF2005] NNNNN> N=15+99 among (Nos 2132-20587).
=E=	Catalogue in electronic form as J/AJ/129/1832
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKF2009]
[GKF2009]	(Greiner+Kruhler+Fynbo+, 2009)
Write:	<<[GKF2009] N>>
N:	9
Object:	* (SIMBAD class: Star)
Note:	MPI/ESO 2.2m telescope GROND optical and NIR photometry.
Ref:	=2009ApJ...693.1610G
by	GREINER J. , KRUHLER T., FYNBO J.P.U., ROSSI A., SCHWARZ R., KLOSE S., SAVAGLIO S., TANVIR N.R., McBREEN S., TOTANI T., ZHANG B.B., WU X.F., WATSON D., BARTHELMY S.D., BEARDMORE A.P., FERRERO P., GEHRELS N., KANN D.A., KAWAI N., KUPCU YOLDAS A., MESZAROS P., MILVANG-JENSEN B., OATES S.R., PIERINI D., SCHADY P., TOMA K., VREESWIJK P.M., YOLDAS A., ZHANG B., AFONSO P., AOKI K., BURROWS D.N., CLEMENS C., FILGAS R., HAIMAN Z., HARTMANN D.H., HASINGER G., HJORTH J., JEHIN E., LEVAN A.J., LIANG E.W., MALESANI D., PYO T.-S., SCHULZE S., SZOKOLY G., TERADA K., WIERSEMA K.
	Astrophys. J., 693, 1610-1620 (2009)
	GRB 080913 at redshift 6.7.
o	Table 2: <[GKF2009] N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKF2010]
[GKF2010]	(Gvaramadze+Kniazev+Fabrika, 2010)
Write:	<<[GKF2010] MNNNN>>
N:	115
Object:	Compact Nebula (SIMBAD class: MidIR = Mid-IR Source (3 to 30 µm))
Stat:	is completely incorporated in Simbad
Note:	N=115 compact nebulae around evolved massive stars, discovered using archival Spitzer MIPS data.
Ref:	=2010MNRAS.405.1047G
by	GVARAMADZE V.V. , KNIAZEV A.Y., FABRIKA S.
	Mon. Not. R. Astron. Soc., 405, 1047-1060 (2010)
	Revealing evolved massive stars with Spitzer.
o	Table 1: <[GKF2010] MNNNN> (Nos MN1-MN115).
=E=	Catalogue in electronic form as <J/MNRAS/405/1047/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKF2018]
[GKF2018]	(Getman+Kuhn+Feigelson+, 2018)
Write:	<<[GKF2018] Be 59 A>> <<[GKF2018] Be 59 UnCl>> <<[GKF2018] SFO 2 A>> <<[GKF2018] SFO 2 UnCl>> <<[GKF2018] NGC NNNN A>> <<[GKF2018] NGC 1333 UnCl>> <<[GKF2018] IC NNNN A>> <<[GKF2018] IC NNNN UnCl>> <<[GKF2018] LkHa101 A>> <<[GKF2018] LkHa101 UnCl>> <<[GKF2018] NGC 2068-2071 A>> <<[GKF2018] NGC 2068-2071 UnCl>> <<[GKF2018] ONC Flank W A>> <<[GKF2018] OMC 2-3 A>> <<[GKF2018] OMC 2-3 UnCl>> <<[GKF2018] Mon R2 A>> <<[GKF2018] Mon R2 UnCl>> <<[GKF2018] GGD 12-15 A>> <<[GKF2018] GGD 12-15 UnCl>> <<[GKF2018] Serpens Main A>> <<[GKF2018] Serpens Main UnCl>> <<[GKF2018] Serpens South A>> <<[GKF2018] Serpens South UnCl>> <<[GKF2018] IRAS 20050+2720 A>> <<[GKF2018] IRAS 20050+2720 UnCl>> <<[GKF2018] Sh 2-106 A>> <<[GKF2018] Sh 2-106 UnCl>> <<[GKF2018] LDN 1251B A>> <<[GKF2018] LDN1251B UnCl>> <<[GKF2018] Cep OB3b A>> <<[GKF2018] Cep OB3b UnCl>> <<[GKF2018] Cep A A>> <<[GKF2018] Cep C UnCl>>
N:	52+19
Object:	Cluster of * + Unclustered stellar structure (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=52 clusters of stars and N=19 unclustered stellar structures in 22 SFiNCS star-forming regions. Use of SPCM data.
Ref:	=2018MNRAS.477..298G
by	GETMAN K.V. , KUHN M.A., FEIGELSON E.D., BROOS P.S., BATE M.R., GARMIRE G.P.
	Mon. Not. R. Astron. Soc., 477, 298-324 (2018)
	Young star clusters in nearby molecular clouds.
o	Tables 2+5: <[GKF2018] Be 59 A> (Nos A-B), <[GKF2018] Be 59 UnCl> N=1, <[GKF2018] SFO 2 A> N=1, <[GKF2018] SFO 2 UnCl> N=1, <[GKF2018] NGC NNNN A> N=2+1, <[GKF2018] NGC 1333 UnCl> N=1, <[GKF2018] IC NNNN A> N=2+2, <[GKF2018] IC NNNN UnCl> N=2, <[GKF2018] LkHa101 A> N=1, <[GKF2018] LkHa101 UnCl> N=1, <[GKF2018] NGC 2068-2071 A> (Nos A-D), <[GKF2018] NGC 2068-2071 UnCl> N=1, <[GKF2018] ONC Flank W A> N=2, <[GKF2018] OMC 2-3 A> (Nos A-D), <[GKF2018] OMC 2-3 UnCl> N=1, <[GKF2018] Mon R2 A> (Nos A-C), <[GKF2018] Mon R2 UnCl> N=1, <[GKF2018] GGD 12-15 A> N=1, <[GKF2018] GGD 12-15 UnCl> N=1, <[GKF2018] Serpens Main A> (Nos A-B), <[GKF2018] Serpens Main UnCl> N=1, <[GKF2018] Serpens South A> (Nos A-D), <[GKF2018] Serpens South UnCl> N=1, <[GKF2018] IRAS 20050+2720 A> (Nos A-E), <[GKF2018] IRAS 20050+2720 UnCl> N=1, <[GKF2018] Sh 2-106 A> (Nos A-D), <[GKF2018] Sh 2-106 UnCl> N=1, <[GKF2018] LDN 1251B A> N=1, <[GKF2018] LDN1251B UnCl> N=1, <[GKF2018] Cep OB3b A> (Nos A-D), <[GKF2018] Cep OB3b UnCl> N=1, <[GKF2018] Cep A A> N=1+2, <[GKF2018] Cep C UnCl> N=1.
=E=	Catalogue in electronic form as <J/MNRAS/477/298/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKG2005]
[GKG2005]	(Gaensler+Kouveliotou+Gelfand+, 2005)= (VLA)
Write:	<<[GKG2005] VLA JHHMMSS+DDMMSS>>
N:	1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA, ATCA, WSST and MOST images are used to study 'NAME SGR 1806-20'. A bright but fading radio source is found.
Ref:	=2005Natur.434.1104G
by	GAENSLER B.M. , KOUVELIOTOU C., GELFAND J.D., TAYLOR G.B., EICHLER D., WIJERS R.A.M., GRANOT J., RAMIREZ-RUIZ E., LYUBARSKY Y.E., HUNSTEAD R.W., CAMPBELL-WILSON D., VAN DER HORST A.J., McLAUGHLIN M.A., FENDER R.P., GARRETT M.A., NEWTON-McGEE K.J., PALMER D.M., GEHRELS N., WOODS P.M.
	Nature, 434, 1104-1106 (2005)
	An expanding radio nebula produced by a giant flare from the magnetar SGR 1806-20.
o	Fig.1: <[GKG2005] VLA JHHMMSS+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKG2008]
[GKG2008]	(Grupe+Komossa+Gallo+, 2008)
Write:	<<[GKG2008] N>>
N:	5
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of Mrk 335. N=5 reference stars.
Ref:	=2008ApJ...681..982G
by	GRUPE D. , KOMOSSA S., GALLO L.C., FABIAN A.C., LARSSON J., PRADHAN A.K., XU D., MINIUTTI G.
	Astrophys. J., 681, 982-997 (2008)
	XMM-Newton observations of the narrow-line Seyfert 1 galaxy Mrk 335 in a historical low X-ray flux state.
o	Table 2: <[GKG2008] N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GKH
GKH	(Gomez+Kenyon+Hartmann)
Note:	Tables 4, 5: (Nos 1-46), N=46 stars
*****	Avoid the usage of GKH, prefer [GKH94]
Origin	of the Acronym: L (1999AJ....117.1471I)
Details on Acronym: [GKH2003]
[GKH2003]	(Gilmore+Kilmartin+Henden, 2003)
Write:	<<[GKH2003] Star A>>
N:	2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Mt John 0.6m telescope and USNO 1.0m telescope observations of GRB 030323. N=2 comparison stars.
Ref:	=2003GCN..1949....1G
by	GILMORE A. , KILMARTIN P., HENDEN A.
	GRB Coordinates Network, Circular Service, 1949, 1-None (2003)
	GRB030323, possible optical counterpart.
o	<[GKH2003] Star A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKH73]
[GKH73]	(Grasdalen+Kuhi+Harlan, 1973)
Write:	<<[GKH73] GLLL.l+BB.b A>>
N:	8
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Note:	Lick Observatory observations of N=8 Hα emission objects in four dust clouds. Use of Palomar Sky Survey prints to estimate positions and magnitudes.
Ref:	=1973PASP...85..193G
by	GRASDALEN G.L. , KUHI L.V., HARLAN E.A.
	Publ. Astron. Soc. Pac., 85, 193-199 (1973)
	New emission-line stars in OH clouds.
o	Plates I-IV, Table II: <[GKH73] GLLL.l+BB.b A> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKH94]
[GKH94]	(Gomez+Kenyon+Hartmann, 1994)= (GKH)
Write:	<<[GKH94] NN>>
N:	46
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Tables 4, 5: (Nos 1-46), N=46 stars
in source:	NAME TMC
Ref:	=1994AJ....107.1850G
by	GOMEZ M. , KENYON S.J., HARTMANN L.
	Astron. J., 107, 1850-1858 (1994)
	A near-infrared survey for pre-main sequence stars in Taurus.
o	E=Elia 3-, T=[TNS87], CIDA=[BCG93]. K=KIM not in SIMBAD
o	Tables 4,5: <[GKH94] NN> N=46
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKJ2003]
[GKJ2003]	(Gordon+Koribalski+Jones, 2003)
Write:	<<[GKJ2003] N>> <<[GKJ2003] ATCA J2001-4650>>
N:	5
Object:	HI G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ATCA HI observations of NGC 6845 group. N=5 HI regions, No. 5 is a previously uncatalogued dwarf galaxy '[GKJ2003] ATCA J2001-4650'.
in source:	NAME NGC 6845 GROUP
Ref:	=2003MNRAS.342..939G
by	GORDON S. , KORIBALSKI B., JONES K.
	Mon. Not. R. Astron. Soc., 342, 939-950 (2003)
	Australia Telescope Compact Array H I observations of the NGC 6845 galaxy group.
o	Fig.2: <[GKJ2003] N> (Nos 1-5), <[GKJ2003] ATCA J2001-4650> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKK2000]
[GKK2000]	(Gouliermis+Kontizas+Korakitis+, 2000)
Write:	<<[GKK2000] NN>>
N:	44
Object:	Assoc. (SIMBAD class: Association = Association of Stars)
Stat:	is completely incorporated in Simbad
Note:	Identification of stellar OB associations in the LMC. See also [GKK2003].
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2000AJ....119.1737G
by	GOULIERMIS D. , KONTIZAS M., KORAKITIS R., MORGAN D.H., KONTIZAS E., DAPERGOLAS A.
	Astron. J., 119, 1737-1747 (2000)
	OB stellar associations in the Large Magellanic Cloud: identification method.
o	Tables 3, 4: <[GKK2000] NN> (Nos 1-44).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKK2003]
[GKK2003]	(Gouliermis+Kontizas+Korakitis, 2003)
Write:	<<[GKK2003] ONNN>> <<[GKK2003] ANNN>>
N:	259+153
Object:	OCl + Assoc. (SIMBAD class: OpenCluster = Open Cluster)
Stat:	is completely incorporated in Simbad
Note:	UK Schmidt Telescope plate digitized by APM. Identification of stellar OB associations and Open clusters in the LMC. In the format the letter 'O' stands for Open cluster, and the letter 'A' for Association. See also [GKK2000].
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2003A&A...405..111G
by	GOULIERMIS D. , KONTIZAS M., KONTIZAS E., KORAKITIS R.
	Astron. Astrophys., 405, 111-124 (2003)
	OB stellar associations in the Large Magellanic Cloud: Survey of young stellar systems.
o	Catalog 1: <[GKK2003] ANNN> (Nos O001-O259). Catalog 2: <[GKK2003] ANNN> (Nos A001-A153).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKK2011]
[GKK2011]	(Gvaramadze+Kniazev+Kroupa+, 2011)
Write:	<<[GKK2011] shell N>>
N:	3
Object:	Circumstellar shell (SIMBAD class: MidIR = Mid-IR Source (3 to 30 µm))
Note:	N=3 circular shells around NGC 6357. Use of Spitzer and 2MASS data.
in source:	NGC 6357
Ref:	=2011A&A...535A..29G
by	GVARAMADZE V.V. , KNIAZEV A.Y., KROUPA P., OH S.
	Astron. Astrophys., 535A, 29-29 (2011)
	Search for OB stars running away from young star clusters. II. The NGC 6357 star-forming region.
o	Figs 13-15, Table 4: <[GKK2011] shell N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GKL
GKL	(Gordon+Kirshner+Long+)
*****	Avoid the usage of GKL, prefer M33SNR
Origin	of the Acronym: L (2001A&A...373..438H)
Details on Acronym: [GKL2003]
[GKL2003]	(Greenhill+Kondratko+Lowell+, 2003)
Write:	<<[GKL2003] JHHMMSS.ss+DDMMSS.s>>
N:	7
Object:	H2O Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	N=7 new H2O masers in 7 galaxies.
in source:	NGC 2824
in source:	NGC 2979
in source:	NGC 5643
in source:	NGC 6926
in source:	ESO 269-12
in source:	IRAS F19370-0131
in source:	NAME Circinus Galaxy
Ref:	=2003ApJ...582L..11G
by	GREENHILL L.J. , KONDRATKO P.T., LOVELL J.E.J., KUIPER T.B.H., MORAN J.M., JAUNCEY D.L., BAINES G.P.
	Astrophys. J., 582, 11-14 (2003)
	The discovery of H_{2}O maser emission in seven active galactic nuclei and at high velocities in the Circinus galaxy.
o	Table 1: <[GKL2003] JHHMMSS.ss+DDMMSS.s> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GKL98
GKL98	(Gordon+Kirshner+Long+, 1998)
*****	Avoid the usage of GKL98, prefer M33SNR
Origin	of the Acronym: L (2001A&A...373..438H)
Details on Acronym: [GKL99]
[GKL99]	(Gershberg+Katsova+Lovkaya+, 1999)
Write:	<<[GKL99] NNN>>
N:	463
Object:	Flare * (SIMBAD class: Eruptive* = Eruptive Variable)
Stat:	is completely incorporated in Simbad
Ref:	=1999A&AS..139..555G
by	GERSHBERG R.E. , KATSOVA M.M., LOVKAYA M.N., TEREBIZH A.V., SHAKHOVSKAYA N.I.
	Astron. Astrophys., Suppl. Ser., 139, 555-558 (1999)
	Catalogue and bibliography of the UV Cet-type flare stars and related objects in the solar vicinity.
o	Table 1: <[GKL99] NNN> (Nos 1-463).
=E=	Catalogue in electronic form as J/A+AS/139/555
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKM2001]
[GKM2001]	(Gonzalez-Perez+Kidger+Martin-Luis, 2001)= (GPK)
Write:	<<[GKM2001] R Zw NNN NN>> <<[GKM2001] NAB HHMM+DD NN>> <<[GKM2001] 3C NNN NN>> <<[GKM2001] 3C NNNA NN>> <<[GKM2001] 3C NNN.N NN>> <<[GKM2001] AO HHMM+DD NN>> <<[GKM2001] PKS HHMM+DD NN>> <<[GKM2001] PKS HHMM+DDd NN>> <<[GKM2001] S5 HHMM+DDd NN>> <<[GKM2001] 87GB HHMMSS.s+DDMMSS NN>> <<[GKM2001] B2 HHMM+DD NN>> <<[GKM2001] OA +NNN NN>> <<[GKM2001] PG HHMM+DDd NN>> <<[GKM2001] Mrk NNN NN>> <<[GKM2001] AA CCC NN>>
N:	432
Object:	* (SIMBAD class: Star)
Note:	Optical and NIR photometry of comparison stars in 26 AGN fields. Finding charts in Figs 4.
Ref:	=2001AJ....122.2055G
by	GONZALEZ-PEREZ J.N. , KIDGER M.R., MARTIN-LUIS F.
	Astron. J., 122, 2055-2098 (2001)
	Optical and near-infrared calibration of AGN field stars: an all-sky network of faint stars calibrated on the Landolt system.
o	Tables 8, 9: <[GKM2001] R Zw NNN NN>, <[GKM2001] NAB HHMM+DD NN>, <[GKM2001] 3C NNN NN>, <[GKM2001] 3C NNNA NN>, <[GKM2001] 3C NNN.N NN>, <[GKM2001] AO HHMM+DD NN>, <[GKM2001] PKS HHMM+DD NN>, <[GKM2001] PKS HHMM+DDd NN>, <[GKM2001] S5 HHMM+DDd NN>, <[GKM2001] 87GB HHMMSS.s+DDMMSS NN>, <[GKM2001] B2 HHMM+DD NN>, <[GKM2001] OA +NNN NN>, <[GKM2001] PG HHMM+DDd NN>, <[GKM2001] Mrk NNN NN>, <[GKM2001] AA CCC NN>, N=432.
=E=	Catalogue in electronic form as J/AJ/122/2055
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKM2012]
[GKM2012]	(Gvaramadze+Kniazev+Miroshnichenko+, 2012)= (WS)
Write:	<<[GKM2012] WSNN>>
N:	about 31
Object:	(MIR) + Shell (SIMBAD class: MidIR = Mid-IR Source (3 to 30 µm))
Note:	Circular shells, detected at 22µm in WISE archival data. In the format, WS stands for "WISE Shell".
Ref:	=2012MNRAS.421.3325G
by	GVARAMADZE V.V. , KNIAZEV A.Y., MIROSHNICHENKO A.S., BERDNIKOV L.N., LANGER N., STRINGFELLOW G.S., TODT H., HAMANN W.-R., GREBEL E.K., BUCKLEY D., CRAUSE L., CRAWFORD S., GULBIS A., HETTLAGE C., HOOPER E., HUSSER T.-O., KOTZE P., LOARING N., NORDSIECK K.H., O'DONOGHUE D., PICKERING T., POTTER S., ROMERO COLMENERO E., VAISANEN P., WILLIAMS T., WOLF M., REICHART D.E., IVARSEN K.M., HAISLIP J.B., NYSEWANDER M.C., LACLUYZE A.P.
	Mon. Not. R. Astron. Soc., 421, 3325-3337 (2012)
	Discovery of two new Galactic candidate luminous blue variables with Wide-field Infrared Survey Explorer.
o	Figs 1-2, Tables 3-4: <[GKM2012] WSN> (Nos WS1-WS2).
Ref:	=2017ASPC..508..207G
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKM2012b]
[GKM2012b]	(Gottschalk+Kothes+Matthews+, 2012)
Write:	<<[GKM2012b] GLL.lll+B.bbb>>
N:	47 (SIMBAD class: Outflow)
Stat:	is completely incorporated in Simbad
Note:	JCMT CO(3-2) observations of the Cygnus X region.
in source:	NAME Cyg X
Ref:	=2012A&A...541A..79G
by	GOTTSCHALK M. , KOTHES R., MATTHEWS H.E., LANDECKER T.L., DENT W.R.F.
	Astron. Astrophys., 541A, 79-79 (2012)
	The JCMT ^{12}CO(3-2) survey of the Cygnus X region. I. A pathfinder.
o	Table 2 : [GKM2012b] GLL.lll+B.bbb N=47
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKM98]
[GKM98]	(Ghez+Klein+Morris+, 1998)
Write:	<<[GKM98] SNN-NNN>>
Object:	* (SIMBAD class: Star)
Note:	The field surrounding Sgr A* is divided into concentric arsecond-wide annuli (from 0 to 17, No. 0 being the central circle). . Stars lying in the central circle, which has a radius of 1", are given the names S0-1, S0-2, S0-3, etc. Stars lying in the annulus between radii of 1"-2" are given the names S1-1, S1-2, and so on. The number immediately following 'S' thus refers to the inner radius of the annulus in which the star lies. The number following the hyphen is ordered in the sense of increasing distance from Sgr A* within each annulus. See also [EG97], [GEO97], [PGM2006], [RGH2007].
in source:	NAME Gal Center
Ref:	=1998ApJ...509..678G
by	GHEZ A.M. , KLEIN B.L., MORRIS M., BECKLIN E.E.
	Astrophys. J., 509, 678-686 (1998)
	High proper-motion stars in the vicinity of Sagittarius A evidence* for a supermassive black hole at the center of our galaxy.
o	cross-id.: WNN = [GEO97] WNN, SNN = [EG97] SNN, NNA or NNWW = GCIRS NNA or NNWW
o	Table 1: <[GKM98] S0-NN> (Nos S0-1 to S0-15), <[GKM98] S1-NN> (Nos S1-1 to S1-15, <[GKM98] S2-NN> (Nos S2-1 to S2-32), <[GKM98] S3-NN> (Nos S3-1 to S3-13), <[GKM98] S4-N> (Nos S4-1 to S4-5).
Ref:	=2002ApJ...576..790G
by	GEZARI S. , GHEZ A.M., BECKLIN E.E., LARKIN J., McLEAN I.S., MORRIS M.
	Astrophys. J., 576, 790-797 (2002)
	Adaptive optics near-infrared spectroscopy of the Sagittarius A* cluster.
o	Table 1, Fig.2: <[GKM98] S0-NN> (Nos S0-16 to S0-18) added.
Ref:	=2003S&T...105d..44T
by	TANNER A.
	Sky Telesc., 105, part no 4, 44-50 (2003)
	A trip to the Galactic Center.
o	Fig.p.49: <[GKM98] SN-NN> (Nos S0-19, S0-20) added.
Ref:	=2005ApJ...620..744G
by	GHEZ A.M. , SALIM S., HORNSTEIN S.D., TANNER A., LU J.R., MORRIS M., BECKLIN E.E., DUCHENE G.
	Astrophys. J., 620, 744-757 (2005)
	Stellar orbits around the Galactic Center black hole.
o	Table 1: <[GKM98] SN-NN> (Nos S0-21 to S0-26) added.
Ref:	=2007ApJ...659.1241R
by	RAFELSKI M. , GHEZ A.M., HORNSTEIN S.D., LU J.R., MORRIS M.
	Astrophys. J., 659, 1241-1256 (2007)
	Photometric stellar variability in the Galactic Center.
o	Tables 2, 3, col(1): <[GKM98] SN-NN> N=69 added among (Nos S0-27 to S0-36, S1-17 to S1-68, S2-34 to S2-86, S3-16). Tables 2, 3, col(2): <[RGH2007] GEN+x.xx+y.yy> N=26.
Ref:	=2007ApJ...667..900H
by	HORNSTEIN S.D. , MATTHEWS K., GHEZ A.M., LU J.R., MORRIS M., BECKLIN E.E., RAFELSKI M., BAGANOFF F.K.
	Astrophys. J., 667, 900-910 (2007)
	A constant spectral index for Sagittarius A during infrared/X-ray* intensity variations.
o	Fig.3: <[GKM98] S0-NN> (No. S0-37) added.
Ref:	=2009ApJ...691.1021D
by	DO T. , GHEZ A.M., MORRIS M.R., YELDA S., MEYER L., LU J.R., HORNSTEIN S.D., MATTHEWS K.
	Astrophys. J., 691, 1021-1034 (2009)
	A near-infrared variability study of the Galactic black hole: a red noise source with NO detected periodicity.
o	Fig.1: <[GKM98] SN-NNN> (Nos S0-38, S2-42, S2-133) added.
Ref:	=2010ApJ...725..331Y
by	YELDA S. , LU J.R., GHEZ A.M., CLARKSON W., ANDERSON J., DO T., MATTHEWS K.
	Astrophys. J., 725, 331-352 (2010)
	Improving Galactic Center astrometry by reducing the effects of geometric distortion.
o	(Erratum) erratum vol. 726, p. 114 (2011)
o	Table 7: <[GKM98] S0-NNN> (Nos S0-53) added, <[GKM98] S1-NNN> (Nos S1-167) added, <[GKM98] S2-NNN> N=9 among (Nos S2-134 to S2-319) added, <[GKM98] S3-NNN> N=81 among (Nos S3-17 to S3-390) added, <[GKM98] S4-NNN> N=77 among (Nos S4-6 to S4-372) added, <[GKM98] S5-NNN> N=86 among (Nos S5-6 to S5-258), <[GKM98] S6-NNN> N=123 among (Nos S6-0 to S6-176), <[GKM98] S7-NNN> N=98 among (Nos S7-3 to S7-103), <[GKM98] S8-NNN> (Nos S8-1 to S8-114), <[GKM98] S9-NNN> (Nos S9-1 to S9-108),<[GKM98] S10-NNN> (Nos S10-1 to S10-95), <[GKM98] S11-NNN> (Nos S11-1 to S11-85), <[GKM98] S12-NNN> (Nos S12-1 to S12-64), <[GKM98] S13-NNN> (Nos S13-1 to S13-60), <[GKM98] S14-NNN> (Nos S14-1 to S14-56), <[GKM98] S15-NNN> (Nos S15-1 to S15-35), <[GKM98] S16-NNN> (Nos S16-1 to S16-18), <[GKM98] S17-NNN> N=10 among (Nos S17-2 to S17-11), <[GKM98] S18-NNN> (Nos S18-1 to S18-3).
Ref:	=2013ApJ...764..154D
by	DO T. , LU J.R., GHEZ A.M., MORRIS M.R., YELDA S., MARTINEZ G.D., WRIGHT S.A., MATTHEWS K.
	Astrophys. J., 764, 154 (2013)
	Stellar populations in the central 0.5 pc of the galaxy. I. A new method for constructing luminosity functions and surface-density profiles.
o	Tables 2-3: <[GKM98] S2-NNN> (Nos S2-317 and S2-319) added, <[GKM98] S6-NNN) (No S6-181) added, <[GKM98] S7-NNN> (No S7-104) added, <[GKM98] S8-NNN> (No S8-124) added, <[GKM98] S11-NNN> (Nos S11-86 and S11-88) added.
Ref:	=2013ApJ...779L...6D
by	DO T. , MARTINEZ G.D., YELDA S., GHEZ A., BULLOCK J., KAPLINGHAT M., LU J.R., PETER A.H.G., PHIFER K.
	Astrophys. J., 779L, 6 (2013)
	Three-dimensional stellar kinematics at the Galactic Center: measuring the nuclear star cluster spatial density profile, black hole mass, and distance.
o	Table 1: <[GKM98] S2-NNN> (Nos S2-308 and S2-317) added, <[GKM98] S6-NNN) (No S6-181) added, <[GKM98] S7-NNN> (No S7-104) added, <[GKM98] S8-NNN> (Nos S8-119, S8-121, S8-124) added, <[GKM98] S10-NNN> N=5 (Nos S10-96 to S10-99, S10-100 to S10-102) added, <[GKM98] S11-NNN> (Nos S11-86 and S11-88) added, <[GKM98] S12-NNN> N=7 among (Nos S12-67 to S12-75) added.
Ref:	=2016ApJ...830...17B
by	BOEHLE A. , GHEZ A.M., SCHODEL R., MEYER L., YELDA S., ALBERS S., MARTINEZ G.D., BECKLIN E.E., DO T., LU J.R., MATTHEWS K., MORRIS M.R., SITARSKI B., WITZEL G.
	Astrophys. J., 830, 17-17 (2016)
	An improved distance and mass estimate for Sgr A from a multistar* orbit analysis.
o	Table 6: <[GKM98] S6-NNN> (Nos S6-182 to S6-185) added, <[GKM98] S7-NNN> (Nos S7-112 and S7-114) added, <[GKM98] S8-NNN> (Nos S8-125 to S8-130) added, <[GKM98] S9-NNN> N=9 among (Nos S9-117 to S9-293) added, <[GKM98] S10-NNN> N=7 among (Nos S10-096 to S10-113) added, <[GKM98] S11-NNN> N=4 among (Nos S11-93 to S11-98) added, <[GKM98] S12-NNN> N=6 among (Nos S12-076 to S12-129) added, <[GKM98] S13-NNN> N=4 among (Nos S13-065 to S13-068) added, <[GKM98] S14-NNN> N=3 among (Nos S14-058 to S14-177) added, <[GKM98] S15-NNN> N=3 among (Nos S15-038 to S15-042) added, <[GKM98] S17-NNN> (No S17-013) added.
=E=	Catalogue in electronic form as J/ApJ/659/1241
=E=	Catalogue in electronic form as <J/ApJ/764/154/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKP2005]
[GKP2005]	(Grant+Kuipers+Phillipps, 2005)
Write:	<<[GKP2005] NNN>> <<[GKP2005] FN>>
N:	181+9
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	INT Virgo survey, using images from the INT WFC survey: N=181 galaxies member of Virgo Cluster, N=9 field galaxies.
in source:	NAME Virgo Cluster
Ref:	=2005MNRAS.363.1019G
by	GRANT N.I. , KUIPERS J.A., PHILLIPPS S.
	Mon. Not. R. Astron. Soc., 363, 1019-1030 (2005)
	Nucleated dwarf elliptical galaxies in the Virgo cluster.
o	In chap. 5.3 : LGC 50 = [FS90] Leo 50
o	Table a1: <[GKP2005] NNN> (Nos 1-181). Table a2 <[GKP2005] FN> (Nos F1-F9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKP2011]
[GKP2011]	(Gerke+Kochanek+Prieto+, 2011)= (M81C)
Write:	<<[GKP2011] M81C JHHMMSS.ss+DDMMSS.s>> <<[GKP2011] M81C HHMMSS.ss+DDMMSS.s>> (not recognised by Simbad, but found in literature)
N:	126
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Note:	LBT observations of N=126 cepheids in M81. Use of HST ACS ANGST (ACS Nearby Galaxy Survey Treasury) data.
in source:	M 81 = NGC 3031
Ref:	=2011ApJ...743..176G
by	GERKE J.R. , KOCHANEK C.S., PRIETO J.L., STANEK K.Z., MACRI L.M.
	Astrophys. J., 743, 176 (2011)
	A study of Cepheids in M81 with the Large Binocular Telescope (efficiently calibrated with Hubble Space Telescope).
o	Table 1: <[GKP2011] M81C JHHMMSS.ss+DDMMSS.s> N=126.
=E=	Catalogue in electronic form as <J/ApJ/743/176/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKP93]
[GKP93]	(Gorham+Kulkarni+Prince, 1993)
Write:	<<[GKP93] HHMM+DDMM>>
N:	8
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 3: N=8 unresolved compact sources
Ref:	=1993AJ....105..314G
by	GORHAM P.W. , KULKARNI S.R., PRINCE T.A.
	Astron. J., 105, 314-319 (1993)
	VLA observations of candidate supernova remnants from the Clark Lake 30.9 MHz galactic plane survey.
o	Table 3: <[GKP93] HHMM+DDMM> N=8
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKS2002]
[GKS2002]	(Green+Kochanek+Siemiginowska+, 2002)
Write:	<<[GKS2002] CXO JHHMMSS.s+DDMMSS>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations in the field of QSO 2345+007. See also [BFK93].
Ref:	=2002ApJ...571..721G
by	GREEN P.J. , KOCHANEK C., SIEMIGINOWSKA A., KIM D.-W., MARKEVITCH M., SILVERMAN J., DOSAJ A., JANNUZI B.T., SMITH C.
	Astrophys. J., 571, 721-732 (2002)
	Chandra observations of the QSO pair Q2345+007: binary or massive dark lens.
o	Table 1: <[GKS2002] CXO JHHMMSS.s+DDMMSS> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKS2003]
[GKS2003]	(Grogin+Koekemoer+Schreier+, 2003)= ([GKS2003a])
Write:	<<[GKS2003] DD.dddddd+DD.dddddd>>
N:	3030
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 catalogue in the CDFS.
in source:	NAME CDFS
Ref:	=2003ApJ...595..685G
by	GROGIN N.A. , KOEKEMOER A.M., SCHREIER E.J., BERGERON J., GIACCONI R., HASINGER G., KEWLEY L., NORMAN C., ROSATI P., TOZZI P., ZIRM A.
	Astrophys. J., 595, 685-697 (2003)
	Hubble Space Telescope imaging in the Chandra Deep Field-South. III. Quantitative morphology of the 1 million second Chandra counterparts and comparison with the field population.
o	Table 1: <[GKS2003] DD.dddddd+DD.dddddd> N=3030.
=E=	Catalogue in electronic form as J/ApJ/595/685
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKS2003a]
[GKS2003a]	(Grogin+Koekemoer+Schreier+, 2003)
*****	Avoid the usage of [GKS2003a], prefer [GKS2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKS2003b]
[GKS2003b]	(Greiner+Klose+Salvato+, 2003)
Write:	<<[GKS2003b] {B\|R\|J}NN>> <<[GKS2003b] Object N>>
N:	11+11+4+3
Object:	* + ? (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Local photometric standards in the field of GRB 011121. 'BNN' for local photometric B, V, 'RNN' for local photometric B, V standards, photometric R(c), (Ic) standards, 'JN' for local photometric in the IR band. In Figs 5, 6, Object 1 and 2 are neighboring objects of GRB and Object 3 is the host galaxy of GRB.
Ref:	=2003ApJ...599.1223G
by	GREINER J. , KLOSE S., SALVATO M., ZEH A., SCHWARZ R., HARTMANN D.H., MASETTI N., STECKLUM B., LAMER G., LODIEU N., SCHOLZ R.-D., STERKEN C., GOROSABEL J., BURUD I., RHOADS J., MITROFANOV I., LITVAK M., SANIN A., GRINKOV V., ANDERSEN M.I., CASTRO CERON J.M., CASTRO-TIRADO A.J., FRUCHTER A., FYNBO J.U., HJORTH J., KAPER L., KOUVELIOTOU C., PALAZZI E., PIAN E., ROL E., TANVIR N.R., VREESWIJK P.M., WIJERS R.A.M.J., VAN DEN HEUVEL E.
	Astrophys. J., 599, 1223-1237 (2003)
	GRB 011121: a collimated outflow into wind-blown surroundings.
o	Table 2: <[GKS2003b] BNN> (Nos B1-B11). Table 3: <[GKS2003b] RNN> (Nos R1-R11). Table 4: <[GKS2003b] JN> (Nos J1-J4). Figs 5, 6: <[GKS2003b] Object N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKS2016]
[GKS2016]	(Grillo+Karman+Suyu+, 2016)
Write:	<<[GKS2016] NNNa>> <<[GKS2016] cNNN>>
N:	134+300
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT MUSE spectroscopy of N=134 sources in the field of the Hubble Frontier Fields (HFF) galaxy cluster MCS J1149.5+2223. Use of CLASH HST photometric data to obtain a catalog of N=300 candidate cluster members (format cNNN)).
in source:	ClG J1149+2223 = MCS J1149.5+2223
Ref:	=2016ApJ...822...78G
by	GRILLO C. , KARMAN W., SUYU S.H., ROSATI P., BALESTRA I., MERCURIO A., LOMBARDI M., TREU T., CAMINHA G.B., HALKOLA A., RODNEY S.A., GAVAZZI R., CAPUTI K.I.
	Astrophys. J., 822, 78-78 (2016)
	The story of supernova "Refsdal" told by MUSE.
o	Table 1: <[GKS2016] NNNa> N=134 among (Nos 1-123). Table 6: <[GKS2016] cNNN> (Nos c1-c300).
=E=	Catalogue in electronic form as <J/ApJ/822/78/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKT97]
[GKT97]	(Georgiev+Karatchentsev+Tikhonov, 1997)
Write:	<<[GKT97] UGC NNNN A>> <<[GKT97] UGC NNNN AN>>
N:	69
Object:	* (SIMBAD class: Star)
Note:	Table 2: N=12 secondary standards stars, format 'A' and N=57 brightest Blue (format 'BN') and Red (format 'RN') stars in 13 UGC galaxies. See also [KKK94], [SKT96], [SKT99].
in source:	UGC 288
in source:	UGC 2905
in source:	UGC 3755
in source:	UGC 3860 = DDO 43
in source:	UGC 3966
in source:	UGC 3974
in source:	UGC 4115
in source:	UGC 5721
in source:	UGC 6554
in source:	UGC 6565
in source:	UGC 6572
in source:	UGC 6817
in source:	UGC 7559
Ref:	=1997PAZh...23..586G
by	GEORGIEV T.B. , KARACHENTSEV I.D., TIKHONOV N.A.
	Pis'ma Astron. Zh., 23, 586-594 (1997)
	Distance moduli for thirteen nearby isolated dwarf galaxies.
o	Table 2: <[GKT97] UGC NNNN A> N=12, <[GKT97] UGC NNNN BN> N=51, <[GKT97] UGC NNNN RN> N=6
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKV2005]
[GKV2005]	(Garrett+Knudsen+Van Der Werf, 2005)
Write:	<<[GKV2005] WSRT JHHMMSS+DDMMSS>> <<[GKV2005] VLA JHHMMSS+DDMMSS>>
N:	4+4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	WSRT and VLA detections of gavitationally lensed radio emission associated with the galaxy [KVK2004] SMM J16359+6612. see also [KVK2004].
Ref:	=2005A&A...431L..21G
by	GARRETT M.A. , KNUDSEN K.K., VAN DER WERF P.P.
	Astron. Astrophys., 431, 21-24 (2005)
	Gravitationally lensed radio emission associated with SMM J16359+6612, a multiply imaged submillimeter galaxy behind A2218.
o	Table 1: <[GKV2005] WSRT JHHMMSS+DDMMSS> N=4, <[GKV2005] VLA JHHMMSS+DDMMSS> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKW2013]
[GKW2013]	(Giacintucci+Kale+Wik+, 2013)
Write:	<<[GKW2013] SN>>
N:	7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	GMRT 610MHz and 235MHz observations of N=7 radio sources in the X-ray luminous galaxy cluster PLCKG 171.9-40.7.
in source:	PLCKESZ G171.9-40.7
Ref:	=2013ApJ...766...18G
by	GIACINTUCCI S. , KALE R., WIK D.R., VENTURI T., MARKEVITCH M.
	Astrophys. J., 766, 18 (2013)
	Discovery of a giant radio halo in a new planck galaxy cluster PLCKG171.9-40.7.
o	(Erratum) erratum vol. 770, art. A161 (2013)
o	Table 3: <[GKW2013] SN> (Nos S1-S7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GKW97]
[GKW97]	(Gomez+Kenyon+Whitney, 1997)
Write:	<<[GKW97] Knot AN>> <<[GKW97] HH 215 N>> <<[GKW97] FS>>
N:	24+5+1
Object:	Jet (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=24 knots in HH 215, N=5 HH/jet emissions flow detected in HH 215, N=1 Field Star 'FS'.
in source:	HH 215
Ref:	=1997AJ....114..265G
by	GOMEZ M. , KENYON S.J., WHITNEY B.A.
	Astron. J., 114, 265-271 (1997)
	The bipolar optical outflow associated with PV Cephei.
o	Table 2, Figs: <[GKW97] Knot AN> N=24, <[GKW97] HH 215 N> (Nos 1-5), <[GKW97] FS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Gl
Gl	(Gliese)
====>	Equivalent to: GJ
Details on Acronym: Gl
Gl	(Gliese)
====>	Equivalent to: GJ
Details on Acronym: GL
GL	(Geophysics Lab.)
*****	Avoid the usage of GL, prefer RAFGL
Details on Acronym: GL1PN
GL1PN	(GLIMPSE-I PN) (Not yet in Simbad)
*****	Avoid the usage of GL1PN, prefer GLIPN
Origin	of the Acronym: L (2014MNRAS.440.1080F)
Details on Acronym: [GL2004]
[GL2004]	(Gutierrez+Lopez-Corredoira, 2004)= [GL2004a]
Write:	<<[GL2004] Object N>> <<[GL2004] Filament>>
N:	4+1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Broadband imaging at the NOT and spectroscopy at the WHT of the region around the NEQ3 system ([A77b] NEQ3). See also [A77b].
Ref:	=2004ApJ...605L...5G
by	GUTIERREZ C.M. , LOPEZ-CORREDOIRA M.
	Astrophys. J., 605, 5-8 (2004)
	QSO+Galaxy association and discrepant redshifts in NEQ3.
o	Fig.1: <[GL2004] Object N> (Nos 1-4), <[GL2004] Filament> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GL2004a]
[GL2004a]	(Gutierrez+Lopez-Corredoira, 2004)
*****	Avoid the usage of [GL2004a], prefer [GL2004]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GL2004b]
[GL2004b]	(Gal+Lubin, 2004)
Write:	<<[GL2004b] J1604+4314 A>>
N:	10
Object:	Cl of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Keck observations. The supercluster ClG J1604+4314 is detected as 10 individual clusters A to J.
in source:	NAME Cl J1604 Supercluster
Ref:	=2004ApJ...607L...1G
by	GAL R.R. , LUBIN L.M.
	Astrophys. J., 607, 1-4 (2004)
	Spectroscopic confirmation of the Cl 1604 supercluster at z~0.9.
o	Cl 1604 supercluster = ClG J1604+4314 = NAME Cl J1604 SUPERCLUSTER in SIMBAD.
o	Table 1: <[GL2004b] J1604+4314 A> (Nos A-D).
Ref:	=2005AJ....129.1827G
by	GAL R.R. , LUBIN L.M., SQUIRES G.K.
	Astron. J., 129, 1827-1831 (2005)
	Pushing the boundaries of the Cl 1604 supercluster at z~0.9.
o	Table 2, Fig.3: <[GL2004b] J1604+4314 A> (Nos E-H) added.
Ref:	=2008ApJ...684..933G
by	GAL R.R. , LEMAUX B.C., LUBIN L.M., KOCEVSKI D., SQUIRES G.K.
	Astrophys. J., 684, 933-956 (2008)
	The complex structure of the Cl 1604 supercluster at z ~ 0.9.
o	Table 1: <[GL2004b] J1604+4314 A> (Nos I-J) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GL2007]
[GL2007]	(Gutierrez+Lopez-Corredoira, 2007) (Not yet in Simbad)
Write:	<<[GL2007] QSO J1225+1813 abs N.NNNN>>
N:	1
Object:	Absorber
Note:	MgII absorber in QSO J1225+1813.
Ref:	=2007A&A...472...87G
by	GUTIERREZ C.M. , LOPEZ-CORREDOIRA M.
	Astron. Astrophys., 472, 87-92 (2007)
	Eight more ultra luminous X-ray candidates unmasked.
o	SW 78 = QSO J1225+1813.
o	Paragr. 3.8: <[GL2007] QSO J1225+1813 abs N.NNNN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GL65]
[GL65]	(Graham+Lynga, 1965)
Write:	<<[GL65] NNN>>
N:	462
Object:	OB* (SIMBAD class: Star)
Note:	Mount Stromlo Schmidt 50/65cm telescope observations of N=462 OB stars in a region of area of approximately 75 square degrees centred in the star ν Carinae.
Ref:	=1965MmMtS..18....0G
by	GRAHAM J.A. , LYNGA G.
	Mem. Mount Stromlo Obs., -1-None (1965)
	A survey of faint OB stars in Carinae (1965).
o	Table 1: <[GL65] NNN> N=454 among (Nos 1-462).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GLARE
GLARE	(Gemini Ly-Alpha Reionisation Era project)
Write:	<<GLARE NNNN>>
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	Gemini observations. The numbering 'NNNN' described in 2007MNRAS.376..727S, is always a 4 digit numbering.
Ref:	=2004ApJ...604L..13S
by	STANWAY E.R. , GLAZEBROOK K., BUNKER A.J., ABRAHAM R.G., HOOK I., RHOADS J., McCARTHY P.J., BOYLE B., COLLESS M., CRAMPTON D., COUCH W., JORGENSEN I., MALHOTRA S., MUROWINSKI R., ROTH K., SAVAGLIO S., TSVETANOV Z.
	Astrophys. J., 604, 13-16 (2004)
	Three Lyα emitters at z ~ 6: early GMOS/Gemini data from the GLARE project.
o	Parag. 5.3 : CDF-S 202 = [GZW2002] XID 202, CXO 52 = CXOU J084837.9+445352
o	<GLARE NNNN> (Nos 1042, 3001, 3011).
Ref:	=2007MNRAS.376..727S
by	STANWAY E.R. , BUNKER A.J., GLAZEBROOK K., ABRAHAM R.G., RHOADS J., MALHOTRA S., CRAMPTON D., COLLESS M., CHIU K.
	Mon. Not. R. Astron. Soc., 376, 727-738 (2007)
	The GLARE Survey - II. Faint z ~ 6 Lyα line emitters in the HUDF.
o	Tables 2-5: <GLARE NNNN> N=21 among (Nos 1001-8005) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Glass
Glass	(Glass)
Write:	<<Glass A>>
N:	22
Object:	* in Assoc. (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 2. Identif. (Plate I)
Ref:	=1979MNRAS.187..305G
by	GLASS I.S.
	Mon. Not. R. Astron. Soc., 187, 305-310 (1979)
	Infrared photometry of stars in the Chamaeleon T association.
o	Table 2: <Glass A> (Nos A-V).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: GLASS
GLASS	(Grism Lens-Amplified Survey from Space)
*****	Avoid the usage of GLASS, prefer [TSB2015]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Glazar
Glazar	(Glazar telescope)= (Cas1) = (Cas2) = (Cru) = (Cyg) = (Gem) = (Mon) = (Ori) = (Per) = (Pup) = (Sco) = (Vel) = (Vela)
Write:	<<Glazar HHMM+DD>> <<Glazar HHMM+DD.N>> <<Glazar CCC NNNa>> <<Glazar CasN NN>>
Object:	* in Assoc. (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Ultraviolet (1640Å) observations with the space telescope `Glazar', survey at high galactic latitudes and investigation of regions of stellar associations. In the format HHMM+DD.N the fraction .N means an insertion, not a decimal. Identif. charts, 1950 coord.
Ref:	=1990Afz....33..329T
by	TOVMASSIAN H.M. , HOVHANNESSIAN R.K., EPREMIAN R.A., HUGUENIN D.
	Astrofizika, 33, 329-None (1990)
	The distribution of early type stars in the direction of stellar associations PER OB1, SCO OB1 and CYG OB1.
o	Table 1: <Glazar Per NN> (Nos 1-42), <Glazar Sco NNa> (Nos 1-20, 4a-4b), <Glazar Cyg NN> (Nos 1-30)
Ref:	=1991Afz....34..301T
by	TOVMASYAN G.M. , OGANESYAN R.K.
	Astrofizika, 34, 301-314 (1991)
	The Orion complex according to observations of the space telescope Glazar.
o	Table 1: Col.(1): <Glazar Ori NNa> (Nos 1-96) N=101, Col(2): <Glazar HHMM+DD> N=1
Ref:	=1991AZh....68..942T
by	TOVMASSIAN H.M. , HOVHANNESSIAN R.K., EPREMIAN R.A., HUGUENIN D., VIKTORENKO A.S., SEREBROV A.A.
	Astron. Zh., 68, 942-958 (1991)
	Observations in the fields of Cassiopea, Gemini and Monoceros with the Glazar space telescope.
o	Table 1, col(1): <Glazar Cas1 N> (Nos 1-7), <Glazar Cas2 NN> (Nos 1-11), <Glazar Gem NN> (Nos 1-13), <Glazar Mon NN> (Nos 1-35). Table 1, col(2) and Table 2: <Glazar HHMM+DD>, <Glazar HHMM+DD.N> N=11
Ref:	=1992Ap&SS.188..217T
by	TOVMASSIAN H.M. , HOVHANNESSIAN R.K., EPREMIAN R.A., HUGUENIN D., KHODJAYANTS Y.M., KRMOYAN M.N., KASHIN A.L., ALEXANDROV A.P., ROMANENKO Y.V.
	Astrophys. Space Sci., 188, 217-231 (1992)
	Ultraviolet observations in Puppis with the Space Telescope 'Glazar'.
o	Table I: <Glazar Pup NNN> (Nos 1-159). Table II, 2eme col. <Glazar HHMM+DD> and <Glazar HHMM+DD.N> N=43
Ref:	=1993A&AS..100..501T
by	TOVMASSIAN H.M. , HOVHANNESSIAN R.K., EPREMIAN R.A., HUGUENIN D.
	Astron. Astrophys., Suppl. Ser., 100, 501-515 (1993)
	Bright blue stars in Vela observed with the "Glazar" space telescope.
o	Table 1, 1ere col.: <Glazar Vel NN> (Nos 1-71), 2eme col.: <Glazar HHMM+DD.N> N=2. Text: <Ass CCC A N.N>, <Ass CCC OB N.N> 1st ref. with this format.
Ref:	=1994MNRAS.266..337T
by	TOVMASSIAN H.M. , HOVHANNESSIAN R.K., EPREMIAN R.A., HUGUENIN D.
	Mon. Not. R. Astron. Soc., 266, 337-342 (1994)
	The distribution of OB stars in the directions of the stellar associations Aur OB 1 and 2.
o	Table 1, 1ere col.: <Glazar Aur NN> (Nos 1-42), 2eme col.: <Glazar HHMM+DD> N=2.
Ref:	=1996AJ....111..299T
by	TOVMASSIAN H.M. , NAVARRO S.G., CARDONA O., HOVHANNESSIAN R.K., EPREMIAN R.A.
	Astron. J., 111, 299-305 (1996)
	OB stellar association in Crux. I. Observations with the Galzar Space Telescope.
o	Table 2: <Glazar Cru NNN> (Nos 1-217)
Ref:	=1998AJ....115.1083T
by	TOVMASSIAN H.M. , EPREMIAN R.A., HOVHANNESSIAN R.K., CRUZ-GONZALEZ G., NAVARRO S.G., KARAPETIAN A.A.
	Astron. J., 115, 1083-1095 (1998)
	OB stellar associations in the direction of Centaurus OB2.
o	Table 1 : the only SAO star is #89 = SAO 252509 (not 251509). Star #1 42 : HD 08970 misprint for 308970.
o	Table 1: <Glazar Cen NNNa> (Nos 1-185) N=190, <Glazar HHMM+DD> and <Glazar HHMM+DD.d> N=6
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GLB2004]
[GLB2004]	(Green+Lacy+Bhatnagar+, 2004)
Write:	<<[GLB2004] 0314+57.8 A>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	GMRT and CLFST observations of WKB 0314+57.8. Use of VLA and WSRT archival data.
Ref:	=2004MNRAS.354.1159G
by	GREEN D.A. , LACY M., BHATNAGAR S., GATES E.L., WARNER P.J.
	Mon. Not. R. Astron. Soc., 354, 1159-1164 (2004)
	Radio and near-infrared observations of the steep-spectrum Galactic plane radio source WKB 0314+57.8.
o	Calibrator 0432+416 = JVAS J0432+416. Standard stars P138C and S754C are GSPC P138-C and GSPC S754-C.
o	Fig.1, Table 1: <[GLB2004] 0314+57.8 A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLB2011]
[GLB2011]	(George+Leauthaud+Bundy+, 2011)
Write:	<<[GLB2011] Group NNN>> <<[GLB2011] COSMOS CL JHHMMSS.s+DDMMSS>> <<[GLB2011] Galaxy NNNNNNN>>
N:	183+183+115844
Object:	Group of G + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Catalogs of N=115844 galaxies, members of N=183 X-ray-selected groups in the COSMOS field.
in source:	NAME COSMOS Field
Ref:	=2011ApJ...742..125G
by	GEORGE M.R. , LEAUTHAUD A., BUNDY K., FINOGUENOV A., TINKER J., LIN Y.-T., MEI S., KNEIB J.-P., AUSSEL H., BEHROOZI P.S., BUSHA M.T., CAPAK P., COCCATO L., COVONE G., FAURE C., FIORENZA S.L., ILBERT O., LE FLOC'H E., KOEKEMOER A.M., TANAKA M., WECHSLER R.H., WOLK M.
	Astrophys. J., 742, 125 (2011)
	Galaxies in X-ray groups. I. Robust membership assignment and the impact of group environments on quenching.
o	Group catalog: <[GLB2011] Group NNN> N=183 among (Nos 11-345), <[GLB2011] COSMOS CL JHHMMSS.s+DDMMSS> N=183. Galaxies: <[GLB2011] Galaxy NNNNNNN> N=115844 among (Nos 2-1443962).
=E=	Catalogue in electronic form as <J/ApJ/742/125/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLB96]
[GLB96]	(Giavalisco+Livio+Bohlin+)
Write:	<<[GLB96] GN>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST observations
Ref:	=1996AJ....112..369G
by	GIAVALISCO M. , LIVIO M., BOHLIN R.C., MACCHETTO F.D., STECHER T.P.
	Astron. J., 112, 369-377 (1996)
	On the morphology of the HST faint galaxies.
o	<[GLB96] GN> (Nos G1-G3)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLB97]
[GLB97]	(Gomez+Ledlow+Burns+, 1997)
Write:	<<[GLB97] ACO 578 NN>> <<[GLB97] ACO 1569 NN>>
N:	74+56
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Galaxies in the fields of ACO 578 and ACO 1569
in source:	ACO 578
in source:	ACO 1569
Ref:	=1997AJ....114.1711G
by	GOMEZ P.L. , LEDLOW M.J., BURNS J.O., PINKNEY J., HILL J.M.
	Astron. J., 114, 1711-1727 (1997)
	The cluster dynamics, x-ray emission, and radio galaxies in Abell 578 and Abell 1569.
o	Table 2: <[GLB97] ACO 578 NN> (Nos 1-74). Table 3: <[GLB97] ACO 1569 NN> (Nos 1-56).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLC2002]
[GLC2002]	(Gahm+Lehtinen+Carlqvist+, 2002)
Write:	<<[GLC2002] Cha III-A>> <<[GLC2002] Cha III-A a>> <<[GLC2002] The Serpentine a>>
N:	6+2+19+17
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Note:	SEST 13CO(1-0) and 18CO(1-0) observations of Cha III.
in source:	NAME Cha III
Ref:	=2002A&A...389..577G
by	GAHM G.F. , LEHTINEN K., CARLQVIST P., HARJU J., JUVELA M., MATTILA K.
	Astron. Astrophys., 389, 577-588 (2002)
	The threaded molecular clumps of Chamaeleon III.
o	Fig.1: <[GLC2002] Cha III-A> (Nos A-F). Table 1: <[GLC2002] Cha III-A a> (Nos a-b), <[GLC2002] Cha III-B a> (Nos a-s), <[GLC2002] The Serpentine a> (Nos a-q).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLC2011]
[GLC2011]	(Gratton+Lucatello+Carretta+, 2011) (Not yet in Simbad)
Write:	<<[GLC2011] NNNNN>>
N:	119
Object:	* (SIMBAD class: Star)
Note:	VLT GIRAFFE observations of N=119 program stars in NGC 2808.
in source:	NGC 2808
Ref:	=2011A&A...534A.123G
by	GRATTON R.G. , LUCATELLO S., CARRETTA E., BRAGAGLIA A., D'ORAZI V., AL MOMANY Y.
	Astron. Astrophys., 534A, 123-123 (2011)
	The Na-O anticorrelation in horizontal branch stars. I. NGC 2808.
o	Tables 1-2: <[GLC2011] NNNNN> N=119 among (Nos 111-63132).
=E=	Catalogue in electronic form as J/A+A/534/A123
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLC2012]
[GLC2012]	(Gratton+Lucatello+Carretta+, 2012)
Write:	<<[GLC2012] NNNNN>>
N:	103
Object:	HB* (SIMBAD class: HorBranch* = Horizontal Branch Star)
Note:	VLT FLAMES observations of N=103 horizontal branch stars in NGC 1851.
in source:	NGC 1851
Ref:	=2012A&A...539A..19G
by	GRATTON R.G. , LUCATELLO S., CARRETTA E., BRAGAGLIA A., D'ORAZI V., AL MOMANY Y., SOLLIMA A., SALARIS M., CASSISI S.
	Astron. Astrophys., 539A, 19-19 (2012)
	The Na-O anticorrelation in horizontal branch stars. II. NGC 1851.
o	(Erratum) + corrigendum vol. 547, p. C2
o	Table 1: <[GLC2012] NNNNN> N=103 among (Nos 3515-54362).
=E=	Catalogue in electronic form as J/A+A/539/A19
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLD2007]
[GLD2007]	(Giannini+Lorenzetti+De Luca+, 2007)
Write:	<<[GLD2007] NN>>
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Spitzer MIPS survey of of the Vela Molecular Ridge VMR D. N=67 SSTVMRD sources detected at 70mu.m.
in source:	VMR D
Ref:	=2007ApJ...671..470G
by	GIANNINI T. , LORENZETTI D., DE LUCA M., NISINI B., MARENGO M., ALLEN L., SMITH H.A., FAZIO G., MASSI F., ELIA D., STRAFELLA F.
	Astrophys. J., 671, 470-482 (2007)
	Spitzer MIPS survey of the young stellar content in the Vela Molecular Ridge-D.
o	Table 2: <SSTVMRD JHHMMSS.s+DDMMSS.s> N=849. Table 3: <[GLD2007] NN> (Nos 1-67).
=E=	Catalogue in electronic form as J/ApJ/671/470
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GLEAM
GLEAM	(GaLactic and Extragalactic All-sky MWA (Survey))
Write:	<<GLEAM JHHMMSS+DDMMSS>>
N:	about 350000 (SIMBAD class: Radio = Radio Source)
Note:	This is the extragalactic radio catalogue from the first year of the GaLactic and Extragalactic All-sky MWA survey, covering almost the entire sky south of Dec +30, to a 5-sigma limit of about 50 mJy at 200MHz. Excluded regions are the Galactic Plane, the Magellanic Clouds, areas around three bright sources, and a small area of the North where ionospheric conditions were unfavourable. The catalogue contains measurements for each source in 20 7.68-MHz sub-bands from 72 to 231 MHz, as well as a fiducial 200-MHz measurement using a 60-MHz bandwidth deep combined image. The resolution is approximately 2 arcminutes; position precision is dominated by ionospheric conditions and we estimate our astrometry to be good to 3 arcsec in the main survey region of -75 < Dec < 20, and 10 arcsec outside this region.
Notes:	The existing publication is the survey description paper: http://arxiv.org/abs/1505.06041, and there will be a paper published specifically devoted to this catalogue in either late 2015 or early 2016. There will then be further publications using more data, or dealing with currently-excluded regions of the sky.
Ref:	=2017MNRAS.464.1146H
by	HURLEY-WALKER N. , CALLINGHAM J.R., HANCOCK P.J., FRANZEN T.M.O., HINDSON L., KAPINSKA A.D., MORGAN J., OFFRINGA A.R., WAYTH R.B., WU C., ZHENG Q., MURPHY T., BELL M.E., DWARAKANATH K.S., FOR B., GAENSLER B.M., JOHNSTON-HOLLITT M., LENC E., PROCOPIO P., STAVELEY-SMITH L., EKERS R., BOWMAN J.D., BRIGGS F., CAPPALLO R.J., DESHPANDE A.A., GREENHILL L., HAZELTON B.J., KAPLAN D.L., LONSDALE C.J., McWHIRTER S.R., MITCHELL D.A., MORALES M.F., MORGAN E., OBEROI D., ORD S.M., PRABU T., UDAYA SHANKAR N., SRIVANI K.S., SUBRAHMANYAN R., TINGAY S.J., WEBSTER R.L., WILLIAMS A., WILLIAMS C.L.
	Mon. Not. R. Astron. Soc., 464, 1146-1167 (2017)
	GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey - I. A low-frequency extragalactic catalogue.
o	<GLEAM JHHMMSS+DDMMSS> N=307455. International Centre for Radio Astronomy Research / Curtin University
=E=	Catalogue in electronic form as VIII/100
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: GLEAM-X
GLEAM-X	(GaLactic and Extragalactic All-sky Murchison Widefield Array survey eXtended) (Not yet in Simbad)
Write:	<<GLEAM-X JHHMMSS.s+DDMMSS>>
N:	78967
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	A low-frequency wideband radio survey of the southern sky with MWA. For more information, visit: https://www.mwatelescope.org/science/galactic-science/gleam-x/ See also GLEAM.
Ref:	=2022PASA...39...35H
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GLF2007]
[GLF2007]	(Gal-Yam+Leonard+Fox+, 2007)
Write:	<<[GLF2007] N>>
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Observations of 9 calibration stars near SN 2005gl at the robotic 1.5m telescope at Palomar Observatory.
Ref:	=2007ApJ...656..372G
by	GAL-YAM A. , LEONARD D.C., FOX D.B., CENKO S.B., SODERBERG A.M., MOON D.-S., SAND D.J., LI W., FILIPPENKO A.V., ALDERING G., COPIN Y.
	Astrophys. J., 656, 372-381 (2007)
	On the progenitor of SN 2005gl and the nature of type IIn supernovae.
o	Fig.6, Table 2: <[GLF2007] N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLF2012]
[GLF2012]	(Gonzales-Nuevo+Lapi+Fleuren+, 2012)= ([GLF2012a])
Write:	<<[GLF2012] SDP NNN lens>> <<[GLF2012] SDP NNN source>>
N:	64+64
Object:	Poss. Grav. lens + G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=64 gravitational lensing candidates and N=64 background sources in the H-ATLAS Science Demonstration Phase (SDP). Use of SDSS and VIKING survey data. See also H-ATLAS, SDP.
Ref:	=2012ApJ...749...65G
by	GONZALEZ-NUEVO J. , LAPI A., FLEUREN S., BRESSAN S., DANESE L., DE ZOTTI G., NEGRELLO M., CAI Z.-Y., FAN L., SUTHERLAND W., BAES M., BAKER A.J., CLEMENTS D.L., COORAY A., DANNERBAUER H., DUNNE L., DYE S., EALES S., FRAYER D.T., HARRIS A.I., IVISON R., JARVIS M.J., MICHALOWSKI M.J., LOPEZ-CANIEGO M., RODIGHIERO G., ROWLANDS K., SERJEANT S., SCOTT D., VAN DER WERF P., AULD R., BUTTIGLIONE S., CAVA A., DARIUSH A., FRITZ J., HOPWOOD R., IBAR E., MADDOX S., PASCALE E., POHLEN M., RIGBY E., SMITH D., TEMI P.
	Astrophys. J., 749, 65 (2012)
	Herschel-ATLAS: toward a sample of ~1000 strongly lensed galaxies.
o	Table 1: <[GLF2012] SDP NNN lens> N=64, <[GLF2012] SDP NNN source> N=64.
=E=	Catalogue in electronic form as <J/ApJ/749/65/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLF2012a]
[GLF2012a]	(Gonzales-Nuevo+Lapi+Fleuren+, 2012)
*****	Avoid the usage of [GLF2012a], prefer [GLF2012]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLF2012b]
[GLF2012b]	(GANESHALINGAM+LI+FILIPPENKO+, 2012)
Write:	<<[GLF2012b] NN>>
N:	30 (SIMBAD class: Star)
Note:	KAIT 76cm telescope observation of SN 2002es.
Ref:	=2012ApJ...751..142G
by	GANESHALINGAM M. , LI W., FILIPPENKO A.V., SILVERMAN J.M., CHORNOCK R., FOLEY R.J., MATHESON T., KIRSHNER R.P., MILNE P., CALKINS M., SHEN K.J.
	Astrophys. J., 751, 142 (2012)
	The low-velocity, rapidly fading type Ia supernova 2002es.
o	Table 1: <[GLF2012b] NN> N=30 (Nos 1-30)
Details on Acronym: GLG
GLG	(Gelfand+Lazio+Gaensler)
Write:	<<GLG NNN>>
N:	405
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA 325MHz radio survey of M 31. The vast majority of the sources are not M 31 members.
Ref:	=2004ApJS..155...89G
by	GELFAND J.D. , LAZIO T.J.W., GAENSLER B.M.
	Astrophys. J., Suppl. Ser., 155, 89-100 (2004)
	A wide-field, low-frequency radio survey of the field of M31. I. Construction and statistical analysis of the source catalog.
o	Table 3: <GLG NNN> (Nos 1-405).
=E=	Catalogue in electronic form as J/ApJS/155/89
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GLH2004]
[GLH2004]	(Greene+Lim+Ho, 2004)
Write:	<<[GLH2004] Mrk 1157 clump>> <<[GLH2004] 2E 0507.8+1626 clump>> <<[GLH2004] MS 0459.5+0327 clump>>
N:	3
Object:	HI G (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	N=3 HI clumps assciated with 3 Seyfert galaxies.
Ref:	=2004ApJS..153...93G
by	GREENE J. , LIM J., HO P.T.P.
	Astrophys. J., Suppl. Ser., 153, 93-117 (2004)
	Evidence for interactions in H I imaging of Seyfert galaxies.
o	Table 4: PGC 212747 is a misprint for PGC 212749
o	Table 4: <[GLH2004] Mrk 1157 clump>, <[GLH2004] 2E 0507.8+1626 clump>, <[GLH2004] MS 0459.5+0327 clump>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLH95]
[GLH95]	(Gibb+Little+Heaton+, 2000)
Write:	<<[GLH95] LBS NN AN>>
N:	13+8+4+2
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Note:	LBS 2-17, 23, 18, and 13, are divided into smaller clumps. See also [PGL2001].
in source:	LDN 1630
Ref:	=1995MNRAS.277..341G
by	GIBB A.G. , LITTLE L.T., HEATON B.D., LEHTINEN K.K.
	Mon. Not. R. Astron. Soc., 277, 341-352 (1995)
	Dense clumps in the L1630 molecular cloud : physical structure and properties.
o	LBS NN = LBS 2-NN in SIMBAD.
o	Figs 2, 3: <[GLH95] LBS 17 AN> (Nos A1, B1-B8, D1-D4). Fig.4: <[GLH95] LBS 23 AN> (Nos A1-A2, C1-C6). Fig.7: <[GLH95] LBS 18 AN> (Nos B1-B4). Fig.8: <[GLH95] LBS 13 AN> (Nos B1-B2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Gliese
Gliese	(Gliese)
====>	Equivalent to: GJ
Details on Acronym: Gliese
Gliese	(Gliese)
====>	Equivalent to: GJ
Details on Acronym: GLIMPSE
GLIMPSE	(Galactic Legacy Infrared Mid-Plane Survey Extraordinaire)
Write:	<<GLIMPSE CNN>>
N:	2
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	Discovery of new globular clusters using Spitzer GLIMPSE data.
Ref:	=2005AJ....129..239K
by	KOBULNICKY H.A. , MONSON A.J., BUCKALEW B.A., DARNEL J.M., UZPEN B., MEADE M.R., BABLER B.L., INDEBETOUW R., WHITNEY B.A., WATSON C., CHURCHWELL E., WOLFIRE M.G., WOLFF M.J., CLEMENS D.P., SHAH R., BANIA T.M., BENJAMIN R.A., COHEN M., DICKEY J.M., JACKSON J.M., MARSTON A.P., MATHIS J.S., MERCER E.P., STAUFFER J.R., STOLOVY S.R., NORRIS J.P., KUTYREV A., CANTERNA R., PIERCE M.J.
	Astron. J., 129, 239-250 (2005)
	Discovery of a new low-latitude Milky way globular cluster using GLIMPSE.
o	<GLIMPSE CNN> (No. C01).
Ref:	=2008A&A...489..583K
by	KURTEV R. , IVANOV V.D., BORISSOVA J., ORTOLANI S.
	Astron. Astrophys., 489, 583-587 (2008)
	Obscured clusters.II. GLIMPSE-C02 - A new metal rich globular cluster in the Milky Way.
o	<GLIMPSE CNN> (No. C02). Table 1: <[KIB2008] N> (Nos 1-3). Catalog: <[KIB2008] xxxx.xxx-yy.yyy> N=7623.
=E=	Catalogue in electronic form as <J/A+A/489/583/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GLIMPSE
GLIMPSE	(Galactic Legacy Infrared Mid-Plane Survey Extraordinaire)
*****	Avoid the usage of GLIMPSE, prefer [MCM2005b]
Origin	of the Acronym: L (2007A&A...475..209K)
Details on Acronym: GLIMPSE
GLIMPSE	(Galactic Legacy Infrared Mid-Plane Survey Extraordinaire)
*****	Avoid the usage of GLIMPSE, prefer SSTGLMA
Origin	of the Acronym: L (2005ApJ...629..512U)
Details on Acronym: GLIMPSE
GLIMPSE	(Galactic Legacy Infrared Mid-Plane Survey Extraordinaire)
*****	Avoid the usage of GLIMPSE, prefer SSTGLMC
Origin	of the Acronym: L (2005ApJ...629..512U)
Details on Acronym: GLIPN
GLIPN	(GLIMPSE-I PN)= (GL1PN)
Write:	<<GLIPN JHHMM+DDMM>> <<GLIPN HHMM+DDMM>> (not recognised by Simbad, but found in literature)
N:	5
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	N=5 PN in the GLIMPSE-I point-source archive.
Ref:	=2012MNRAS.427.3016P
by	PARKER Q.A. , COHEN M., STUPAR M., FREW D.J., GREEN A.J., BOJICIC I., GUZMAN-RAMIREZ L., SABIN L., VOGT F.
	Mon. Not. R. Astron. Soc., 427, 3016-3028 (2012)
	Discovery of planetary nebulae using predictive mid-infrared diagnostics.
o	Fig. 1, Tables 2-3+6-7: <GLIPN JHHMM+DDMM> N=5.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GLK96]
[GLK96]	(Geisler+Lee+Kim, 1996)
Write:	<<[GLK96] NNNN>>
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	The complete list of globular clusters seems to contain 9992 objects or more. Some objects are first found in 1996AJ....111.1529G, but others are also found in 1998AJ....115.2337S, 2000AJ....120.2928Z, 2003ApJ...591..850C.
in source:	NGC 4472 = M 49
Ref:	=1996AJ....111.1529G
by	GEISLER D. , LEE M.G., KIM E.
	Astron. J., 111, 1529-1550 (1996)
	Washington photometry of the globular cluster system of NGC 4472. I. Analysis of the metallicities.
o	Table 1: <[GLK96] NNNN> N=222 among (Nos 56-9748)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GLL
GLL	(Gonzalez-Lopezlira+Lomeli-Nunez)
Write:	<<GLL JHHMMSS+DDMMSS>>
N:	39+2
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	CFHT WIRCAM observations of N=39 globular cluster candidates in NGC 4258. 2019ApJ...876...39G: N=2 additional sources. Use of archival optical CFHT MegaCam images.
in source:	NGC 4258
Ref:	=2017ApJ...835..184G
by	GONZALEZ-LOPEZLIRA R.A. , LOMELI-NUNEZ L., ALAMO-MARTINEZ K., ORDENES-BRICENO Y., LOINARD L., GEORGIEV I.Y., MUNOZ R.P., PUZIA T.H., BRUZUAL G.A., GWYN S.
	Astrophys. J., 835, 184-184 (2017)
	The relation between globular cluster systems and supermassive black holes in spiral galaxies: the case study of NGC 4258.
o	Tables 6-7: <GLL JHHMMSS+DDMMSS> N=39.
Ref:	=2019ApJ...876...39G
by	GONZALEZ-LOPEZLIRA R.A. , MAYYA Y.D., LOINARD L., ALAMO-MARTINEZ K., HEALD G., GEORGIEV I.Y., ORDENES-BRICENO Y., LANCON A., LARA-LOPEZ M.A., LOMELI-NUNEZ L., BRUZUAL G., PUZIA T.H.
	Astrophys. J., 876, 39-39 (2019)
	Spectroscopy of NGC 4258 globular cluster candidates: membership confirmation and kinematics.
o	Table 2: <[GML2019] JHHMMSS+DDMMSS> N=11, <GLL JHHMMSS+DDMMSS> N=2 added.
=E=	Catalogue in electronic form as <J/ApJ/835/184/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GLL2005]
[GLL2005]	(Graham+Li+LOSS, 2005)
Write:	<<[GLL2005] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	LOSS observations on KAIT. Host galaxy of SN 2005AR.
Ref:	=2005IAUC.8493....1G
by	GRAHAM J. , LI W.
	IAU Circ., 8493, 1-None (2005)
	Supernova 2005ar.
o	<[GLL2005] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLM2015]
[GLM2015]	(Geller+Latham+Mathieu, 2015)= (WOCS)
Write:	<<[GLM2015] WOCS NNNNN>>
N:	1271
Object:	* (SIMBAD class: Star)
Note:	Radial velocity measurements of N=1271 stars in M67, as part of the WIYN Open Cluster Study (WOCS). See also [HGM2009b], [GMB2010], [GMB2010a] and [TGM2014].
in source:	M 67 = NGC 2682
Ref:	=2015AJ....150...97G
by	GELLER A.M. , LATHAM D.W., MATHIEU R.D.
	Astron. J., 150, 97 (2015)
	Stellar radial velocities in the old open cluster M67 (NGC 2682). I. Memberships, binaries, and kinematics.
o	Table 2: <[GLM2015] WOCS NNNNN> N=1271 among (Nos 1001-37055).
o	p.6: The object 2038 (S2312 = Cl* NGC 2682 Sand 2312) is not in Simbad (no coordinates).
=E=	Catalogue in electronic form as J/AJ/150/97
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLM2016]
[GLM2016]	(Gong+Liu+Maccarone, 2016) (Not yet in Simbad)
Write:	<<[GLM2016] JDDD.ddddd+DD.ddddd>>
N:	119
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	N=119 unique luminous X-ray source candidates with L_X>3.10⁴⁰erg/s from 93 galaxies. Use of Chandra archival data.
Ref:	=2016ApJS..222...12G
by	GONG H. , LIU J., MACCARONE T.
	Astrophys. J., Suppl. Ser., 222, 12 (2016)
	An extreme luminous X-ray source catalog based on Chandra ACIS observations.
o	Table 1: <[GLM2016] DDD.ddddd+DD.ddddd> N=119.
=E=	Catalogue in electronic form as <J/ApJS/222/12/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLM2019]
[GLM2019]	(Garofali+Levesque+Massey+, 2019)
Write:	<<[GLM2019] N604-WRX>> <<[GLM2019] N604-WRXa>>
N:	1+3
Object:	(X) + (Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Gemini GMOS-N observations of N=1 colliding-wind binary (CWB) candidate and N=3 candidate optical counterparts in the HII region NGC 604 of M 33. Use of archival Chandra, XMM-Newton, and HST data.
in source:	NGC 598 = M 33
in source:	M 33:NGC 604 = NGC 604
Ref:	=2019ApJ...880....8G
by	GAROFALI K. , LEVESQUE E.M., MASSEY P., WILLIAMS B.F.
	Astrophys. J., 880, 8-8 (2019)
	The first candidate colliding-wind binary in M33.
o	<[GLM2019] N604-WRX> N=1. Fig. 2, Table 3: <[GLM2019] N604-WRXa> (Nos N604-WRXa to N604-WRXc).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GLMA
GLMA	(Galactic Legacy infrared Mid-Plane survey, Archive)
*****	Avoid the usage of GLMA, prefer SSTGLMA
Origin	of the Acronym: L (2006ApJ...638..241E)
Details on Acronym: GLMC
GLMC	(Galactic Legacy infrared Mid-Plane survey, Catalog)
*****	Avoid the usage of GLMC, prefer SSTGLMC
Origin	of the Acronym: L (2006ApJ...638..241E)
Details on Acronym: GLMP
GLMP	(Garcia-Lario+Manchado+Pych or Pottasch)
Write:	<<GLMP NNNN>>
N:	324
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	See also paper II: [GMP90]
Ref:	=1997A&AS..126..479G
by	GARCIA-LARIO P. , MANCHADO A., PYCH W., POTTASCH S.R.
	Astron. Astrophys., Suppl. Ser., 126, 479-502 (1997)
	Near infrared photometry of IRAS sources with colours like planetary nebulae. III.
o	Table 6: <GLMP NNNN> N=324 among (Nos 9-1083).
=E=	Catalogue in electronic form as J/A+AS/126/479
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Globulette
Globulette	(GLobulette)
*****	Avoid the usage of Globulette, prefer [GGF2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GLOSTAR
GLOSTAR	(Global View of Star Formation in the Milky Way)
Write:	<<GLOSTAR GLLL.lll+BB.bbb>> <<GLOSTAR GLLL.llll+BB.bbbb>>
N:	1575+80+14
Object:	(Rad) + Poss. SNR + Maser (SIMBAD class: Radio = Radio Source)
Note:	Jansky VLA C band observations as part of the Global view on the Star formation in the Milky Way (GLOSTAR) survey. 2019A&A...627A.175M: Catalog of N=1575 radio sources. 2021A&A...651A..86D: N=80 SNR candidates. 2021A&A...651A..87O: N=14 methanol masers. For more information, visit: https://glostar.mpifr-bonn.mpg.de/glostar/
Ref:	=2019A&A...627A.175M
by	MEDINA S.-N.X. , URQUHART J.S., DZIB S.A., BRUNTHALER A., COTTON B., MENTEN K.M., WYROWSKI F., BEUTHER H., BILLINGTON S.J., CARRASCO-GONZALEZ C., CSENGERI T., GONG Y., HOFNER P., NGUYEN H., ORTIZ-LEON G.N., OTT J., PANDIAN J.D., ROY N., SARKAR E., WANG Y., WINKEL B.
	Astron. Astrophys., 627A, 175-175 (2019)
	GLOSTAR: Radio Source Catalog. I. 28° < l < 36° and \|b\| < 1°.
o	Table 7: <GLOSTAR GLLL.lll+BB.bbb> N=1575.
Ref:	=2021A&A...651A..86D
by	DOKARA R. , BRUNTHALER A., MENTEN K.M., DZIB S.A., REICH W., COTTON W.D., ANDERSON L.D., CHEN C.-H.R., GONG Y., MEDINA S.-N.X., ORTIZ-LEON G.N., RUGEL M., URQUHART J.S., WYROWSKI F., YANG A.Y., BEUTHER H., BILLINGTON S.J., CSENGERI T., CARRASCO-GONZALEZ C., ROY N.
	Astron. Astrophys., 651A, 86-86 (2021)
	A global view on star formation: The GLOSTAR Galactic plane survey. II. Supernova remnants in the first quadrant of the Milky Way.
o	Table 3: <GLOSTAR GLLL.lll+BB.bbb> N=80.
Ref:	=2021A&A...651A..87O
by	ORTIZ-LEON G.N. , MENTEN K.M., BRUNTHALER A., CSENGERI T., URQUHART J.S., WYROWSKI F., GONG Y., RUGEL M.R., DZIB S.A., YANG A., NGUYEN H., COTTON W.D., MEDINA S.N.X., DOKARA R., KONIG C., BEUTHER H., PANDIAN J.D., REICH W., ROY N.
	Astron. Astrophys., 651A, 87-87 (2021)
	A global view on star formation: the GLOSTAR Galactic plane survey. III. 6.7 GHz methanol maser survey in Cygnus X.
o	Tables 2-6: <GLOSTAR GLLL.llll+BB.bbbb> N=14.
=E=	Catalogue in electronic form as <J/A+A/627/A175/>
=E=	Catalogue in electronic form as <J/A+A/651/A86/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GLR2008]
[GLR2008]	(Grillo+Lombardi+Rosati+, 2008)
Write:	<<[GLR2008] J0152-1357 lens>> <<[GLR2008] J0152-1357 AN>>
N:	1+4+6
Object:	G + Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	HAST ACS observations. Gravitational lens system in ClG J0152-1357.
Ref:	=2008A&A...486...45G
by	GRILLO C. , LOMBARDI M., ROSATI P., BERTIN G., GOBAT R., DEMARCO R., LIDMAN C., MOTTA V., NONINO M.
	Astron. Astrophys., 486, 45-53 (2008)
	A twelve-image gravitational lens system in the z≃0.84 cluster Cl J0152.7-1357.
o	lens galaxy is [JBD2005] 523
o	Table 1: <[GLR2008] J0152-1357 lens> N=1. Table 2, Fig.1: <[GLR2008] J0152-1357 A> (Nos A-D). Table 3: <[GLR2008] J0152-1357 AN> (Nos A1-A3, B1-B3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLR2016]
[GLR2016]	(Gruyters+Lind+Richard+, 2016)
Write:	<<[GLR2016] NGC 7099 NNNNNN>>
N:	144
Object:	* (SIMBAD class: Star)
Note:	VLT FLAMES GIRAFFE spectroscopic observations of N=144 stars of the globular cluster M30.
in source:	NGC 7099 = M 30
Ref:	=2016A&A...589A..61G
by	GRUYTERS P. , LIND K., RICHARD O., GRUNDAHL F., ASPLUND M., CASAGRANDE L., CHARBONNEL C., MILONE A., PRIMAS F., KORN A.J.
	Astron. Astrophys., 589A, 61-61 (2016)
	Atomic diffusion and mixing in old stars. VI. The lithium content of M30.
o	Table 1: <[GLR2016] NGC 7099 NNNNNN> N=144 among (Nos 36-202112).
=E=	Catalogue in electronic form as J/A+A/589/A61
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Gls
Gls	(Gliese+)
====>	Equivalent to: GJ
Origin	of the Acronym: L (2001MNRAS.325..343M)
Details on Acronym: [GLS2013]
[GLS2013]	(Gratton+Lucatello+Sollima+, 2013)
Write:	<<[GLS2013] 47 Tuc NNNNNN>> <<[GLS2013] M5 NNNNN>>
N:	110+91
Object:	HB* (SIMBAD class: HorBranch* = Horizontal Branch Star)
Note:	VLT GIRAFFE observations of N=110 red HB stars in 47 Tuc and of 61 blue HB and 30 red HB in M5.
in source:	NGC 104 = 47 Tuc
in source:	M 5 = NGC 5904
Ref:	=2013A&A...549A..41G
by	GRATTON R.G. , LUCATELLO S., SOLLIMA A., CARRETTA E., BRAGAGLIA A., MOMANY Y., D'ORAZI V., CASSISI S., PIETRINFERNI A., SALARIS M.
	Astron. Astrophys., 549A, 41-41 (2013)
	The Na-O anticorrelation in horizontal branch stars. III. 47 Tucanae and M 5.
o	Tables 2+4+5: <[GLS2013] 47 Tuc NNNNNN> N=110 among (Nos 341-114008). Tables 3+6: <[GLS2013] M5 NNNNN> N=91 among (Nos 262-42443).
=E=	Catalogue in electronic form as J/A+A/549/A41
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLS2014]
[GLS2014]	(Gratton+Lucatello+Sollima+, 2014)
Write:	<<[GLS2014] NNN>>
N:	92
Object:	HB* (SIMBAD class: HorBranch* = Horizontal Branch Star)
Note:	VLT FLAMES GIRAFFE spectroscopy of N=92 stars in the globular cluster M22.
in source:	M 22 = NGC 6656
Ref:	=2014A&A...563A..13G
by	GRATTON R.G. , LUCATELLO S., SOLLIMA A., CARRETTA E., BRAGAGLIA A., MOMANY Y., D'ORAZI V., CASSISI S., SALARIS M.
	Astron. Astrophys., 563A, 13-13 (2014)
	The Na-O anticorrelation in horizontal branch stars. IV. M 22.
o	Tables 3-6: <[GLS2014] NNN> N=92 among (Nos 1-129).
=E=	Catalogue in electronic form as J/A+A/563/A13
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLS2015]
[GLS2015]	(Gratton+Lucatello+Sollima+, 2015)
Write:	<<[GLS2015] NNNNN>>
N:	51
Object:	HB* (SIMBAD class: Star)
Note:	VLT FLAMES GIRAFFE spectroscopy of N=30 red horizontal branch (RHB) stars + 4 RR Lyrae variables + 17 blue horizontal branch (BHB) stars in the moderately metal-rich globular cluster NGC 6723.
in source:	NGC 6723
Ref:	=2015A&A...573A..92G
by	GRATTON R.G. , LUCATELLO S., SOLLIMA A., CARRETTA E., BRAGAGLIA A., MOMANY Y., D'ORAZI V., SALARIS M., CASSISI S., STETSON P.B.
	Astron. Astrophys., 573A, 92-92 (2015)
	The Na-O anticorrelation in horizontal branch stars. V. NGC 6723.
o	Tables 2-3,5,7-8): <[GLS2015] NNNNN> N=51 among (Nos 32170-77469).
=E=	Catalogue in electronic form as J/A+A/573/A92
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLS2021]
[GLS2021]	(Ge+Luo+Sun+, 2021)
Write:	<<[GLS2021] ACO 1367 Orphan Cloud>>
N:	1
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton and VLT MUSE observations of N=1 orphan cloud detected in the nearby cluster ACO 1367.
in source:	ACO 1367
Ref:	=2021MNRAS.505.4702G
by	GE C. , LUO R., SUN M., YAGI M., JACHYM P., BOSELLI A., FOSSATI M., NULSEN P.E.J., SARAZIN C., EDGE T., GAVAZZI G., GASPARI M., KODA J., KOMIYAMA Y., YOSHIDA M.
	Mon. Not. R. Astron. Soc., 505, 4702-4716 (2021)
	An H α/X-ray orphan cloud as a signpost of intracluster medium clumping.
o	Fig. 2, Table 1: <[GLS2021] ACO 1367 Orphan Cloud> N=1.
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [GLT2000]
[GLT2000]	(Grupe+Leighly+Thomas+, 2000)
Write:	<<[GLT2000] N>>
N:	4
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC and ASCA image of RX J0134.2-4258. N=4 sources are found in the field of the RX.
Ref:	=2000A&A...356...11G
by	GRUPE D. , LEIGHLY K.M., THOMAS H.-C., LAURENT-MUEHLEISEN S.A.
	Astron. Astrophys., 356, 11-22 (2000)
	The enigmatic soft X-ray AGN RX J0134.2-4258.
o	Table 3: <[GLT2000] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLT2013]
[GLT2013]	(Grebenev+Lutovinov+Tsygankov+, 2013)
Write:	<<[GLT2013] JHHMMSS.s+DDMMSS>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Swift XRT observations of N=3 soft X-ray sources in the fields of IGR J05099-6913 and IGR J04288-6702.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2013MNRAS.428...50G
by	GREBENEV S.A. , LUTOVINOV A.A., TSYGANKOV S.S., MEREMINSKIY I.A.
	Mon. Not. R. Astron. Soc., 428, 50-57 (2013)
	Deep hard X-ray survey of the Large Magellanic Cloud.
o	Paragr. 3: <[GLT2013] JHHMMSS.s+DDMMSS> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GLV95]
[GLV95]	(Gry+Lemonon+Vidal-Madjar+, 1995)
Write:	<<[GLV95] N>>
N:	6
Object:	Cloud (SIMBAD class: Cloud)
Note:	HST GHRS observations. Detection of 3 main clouds (Nos 1-3) and 3 weaker (Nos 0, 4-5). No. 1 = Local Interstellar Cloud No. 2 = Blue Component
Ref:	=1995A&A...302..497G
by	GRY C. , LEMONON L., VIDAL-MADJAR A., LEMOINE M., FERLET R.
	Astron. Astrophys., 302, 497-508 (1995)
	The interstellar void in the direction to ε CMa: local clouds and hot gas.
o	Fig.5: <[GLV95] N> (Nos 0-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GLXY
GLXY	(Galaxy, X. Y)
Write:	<<GLXY GLLL.l+BB.b+VVV>>
N:	41+4
Object:	G (SIMBAD class: Galaxy)
Note:	Galaxies found in the catalogue of southern anomalous-velocity HI Clouds. See [PDS2002].
Ref:	=2002AJ....123..873P
by	PUTMAN M.E. , DE HEIJ V., STAVELEY-SMITH L., BRAUN R., FREEMAN K.C., GIBSON B.K., BURTON W.B., BARNES D.G., BANKS G.D., BHATHAL R., DE BLOK W.J.G., BOYCE P.J., DISNEY M.J., DRINKWATER M.J., EKERS R.D., HENNING P.A., JERJEN H., KILBORN V.A., KNEZEK P.M., KORIBALSKI B., MALIN D.F., MARQUARDING M., MINCHIN R.F., MOULD J.R., OOSTERLOO T., PRICE R.M., RYDER S.D., SADLER E.M., STEWART I., STOOTMAN F., WEBSTER R.L., WRIGHT A.E.
	Astron. J., 123, 873-891 (2002)
	HIPASS high-velocity clouds: properties of the compact and extended populations.
o	Table 1, col(1): <[PDS2002] HIPASS HVC NNNN> (Nos 1-1997). Table 3, col(1): <[PDS2002] XHVC NNN> (Nos 1-190). Tables 1, 3, col(2): <GLXY GLLL.l+BB.b+VVV> N=41+4.
=E=	Catalogue in electronic form as J/AJ/123/873
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GM
GM	(Gyulbudaghian+Maghakian)
Write:	<<GM 1-NN>> <<GM 2-NN>> <<GM 3-NN>>
N:	79+42+15
Object:	Nebula + HH-like (SIMBAD class: RefNeb = Reflection Nebula)
Note:	1977PAZh....3..113G: format '1-NN': Table I: (Nos 1-12), Arcuate Nebulae. Table II: (Nos 13-32), Conical Nebulae. Table III: (Nos 33-54), Stars with tailed Nebulae. Table IV: (Nos 55-57), Biconical Nebulae. Table V: (Nos 58-79), Stars in Halo Nebulae. GM 1-29 is a variable cometary nebula illuminated by PV Cep. GM 1-11 is a poss. PN in Gasparian+ 1988Afz....28..679G, and in ref. 1992ESOPN...1....1A. 1977DoArm..64..104G: format '2-NN: Table I: (Nos 1-36) are Herbig-Haro like objects identical to GGD Table II: (Nos 37-44) are Nebular knots in nebulae. 1977ATsir.953....1G: format '3-NN': Neb. objects (Nos 1-15).
Ref:	=1977PAZh....3..113G
by	GYULBUDAGHIAN A.L. , MAGHAKIAN T.Y.
	Pis'ma Astron. Zh., 3, 113-116 (1977)
	New cometary nebulae.
o	Translation in 1977SvAL....3...58G.
o	Tables I-V: <GM 1-NN> (Nos 1-79).
Ref:	=1977DoArm..64..104G
by	GYULBUDAGHIAN A.L. , MAGHAKIAN T.Y.
	Doklady - Akad. Nauk Arm. SSR, 64, 104-107 (1977)
	New red objects resembling Herbig-Haro objects.
o	Tables I-II: <GM 2-NN> (Nos 1-42)
Ref:	=1977ATsir.953....1G
by	GYULBUDAGHIAN A.L. , MAGHAKIAN T.Y.
	Astron. Tsirk., 953, 1-2 (1977)
	New interesting nebulous objects.
o	<GM 3-NN> (Nos 1-15)
Details on Acronym: GM
GM	(Gomez+Mendoza)
*****	Avoid the usage of GM, prefer [GM76]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: GM
GM	(Gallagher+Mould)
*****	Avoid the usage of GM, prefer [GM81]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GM2000]
[GM2000]	(Gomez+Marscher, 2000)= ([GM2000a]) (Not yet in Simbad)
Write:	<<[GM2000] 3C 371 A>> <<[GM2000] 3C 371 KN>>
N:	4+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Fig2, Table 1: N=4 components of 3C 371, (Nos A-D). N=2 knots in 3C 371, (Nos K1-K2).
in source:	3C 371
Ref:	=2000ApJ...530..245G
by	GOMEZ J.-L. , MARSCHER A.P.
	Astrophys. J., 530, 245-250 (2000)
	Space VLBI observations of 3C 371.
o	Fig2, Table 1: <[GM2000] 3C 371 A> (Nos A-D), <[GM2000] 3C 371 KN> (Nos K1-K2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GM2000a]
[GM2000a]	(Gomez+Marscher, 2000) (Not yet in Simbad)
*****	Avoid the usage of [GM2000a], prefer [GM2000]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GM2000b]
[GM2000b]	(Geffert+Maintz, 2000)
Write:	<<[GM2000b] JHHMMSS.sss+DDMMSS.ss>>
N:	4450
Object:	* in Cl* (SIMBAD class: Star)
in source:	M 71 = NGC 6838
Ref:	=2000A&AS..144..227G
by	GEFFERT M. , MAINTZ G.
	Astron. Astrophys., Suppl. Ser., 144, 227-233 (2000)
	First results of a photometric and astrometric study of the globular cluster M 71 (NGC 6838).
o	Table 2: <[GM2000b] JHHMMSS.sss+DDMMSS.ss> N=4450.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GM2006]
[GM2006]	(Gyulbudaghian+May, 2006) (Not yet in Simbad)
Write:	<<[GM2006] NN>> <<[GM2006] SNO 85 NN>> <<[GM2006] SNO NN a>>
N:	14
Object:	* (SIMBAD class: Star)
Note:	SEST observations at Cerro La Silla.
in source:	LDN 288:[GMG2004] 85 = [GMG2004] 85
in source:	LDN 288:[GMG2004] 35 = [GMG2004] 35
in source:	LDN 288:[GMG2004] 69 = [GMG2004] 69
Ref:	=2006Ap.....49..530G
by	GYULBUDAGHIAN A.L. , MAY J.
	Ap, 49, 530-537 (2006)
	An Interesting Nebular Object in LDN 288.
o	Table 1, col(1): <[GM2006] NN> (Nos 1-14) = Table 1, col(2): <[GM2006] SNO 85 AN> (Nos N1-N7), <[GM2006] SNO 35 a> (Nos a-c), <[GM2006] SNO 69 a> (Nos a-f).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GM2007]
[GM2007]	(Gyulbudaghian+May, 2007) (Not yet in Simbad)
Write:	<<[GM2007] NN>> <<[GM2007] SNO 41 a>>
N:	7
Object:	* (SIMBAD class: Star)
Note:	Star formation region connectedwith [GMG2004] 41.
Ref:	=2007Ap.....50....1G
by	GYULBUDAGHIAN A.L. , MAY J.
	Ap, 50, 1-9 (2007)
	Star Formation Region in Vela.
o	Fig.6, Table 1: <[GM2007] SNO 41 a> (Nos a-f).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GM2008]
[GM2008]	(Gyulbudaghian+May, 2008)
Write:	<<[GM2008] cloud N>> <<[GM2008] N>>
N:	2+9
Object:	MCld + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	SEST SIMBA observations of the RCW 38 IR Cluster. Use of 2MASS archival data.
in source:	NAME RCW 38 IR Cluster
Ref:	=2008Ap.....51...18G
by	GYULBUDAGHIAN A.L. , MAY J.
	Ap, 51, 18-28 (2008)
	Investigation of the conspicuous infrared star cluster and star-forming region "RCW 38 IR Cluster".
o	Text: <[GM2008] cloud N> (Nos 1-2). Table 2: <[GM2008] N> (Nos 1-9).
o	A translation of Astrofizika Vol. 51, No 1, pp.29-40, 2008
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GM2010]
[GM2010]	(Gyulbudaghian+May, 2010) (Not yet in Simbad)
Write:	<<[GM2010] GRV10 IR>>
N:	1
Object:	* (SIMBAD class: Star)
Note:	N=1 bright IR star near the southern edge of the nebula [GRV93] 10.
Ref:	=2010Ap.....53..503G
by	GYULBUDAGHIAN A.L. , MAY J.
	Ap, 53, 503-510 (2010)
	Southern YSO GRV 10 and its environment.
o	<[GM2010] GRV10 IR> N=1.
o	A translation of Astrofizika Vol. 53, No 4, pp. 565-573, 2010 Table 2 NN13 star 3 is NOMAD1 0714-0136444.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GM2013]
[GM2013]	(Graur+Maoz, 2013)
Write:	<<[GM2013] SDSS NNNN-NNNNN-NNN SN>>
N:	100
Object:	SN (SIMBAD class: Supernova = SuperNova)
Note:	N=100 supernovae discovered in SDSS DR7 galaxy spectra.
Ref:	=2013MNRAS.430.1746G
by	GRAUR O. , MAOZ D.
	Mon. Not. R. Astron. Soc., 430, 1746-1763 (2013)
	Discovery of 90 Type Ia supernovae among 700 000 Sloan spectra: the Type Ia supernova rate versus galaxy mass and star formation rate at redshift ~ 0.1.
o	Table 4 : no coordinates are provided for the SNe; ingested in SIMBAD with the coordinates of the Galaxy truncated to 1''.
o	Table 4: <[GM2013] SDSS NNNN-NNNNN-NNN SN> N=100.
=E=	Catalogue in electronic form as <J/MNRAS/430/1746/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GM76]
[GM76]	(Gomez+Mendoza, 1976)= (GM)
Write:	<<[GM76] NNN>>
N:	275
Object:	Em. Obj. (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Note:	Identif. charts
Ref:	=1976RMxAA...1..381G
by	GOMEZ T. , MENDOZA V E.E.
	Rev. Mex. Astron. Astrofis., 1, 381-384 (1976)
	A finding list of H alf-emission objects in the Coalsack direction.
o	Table 1: <[GM76] NNN> (Nos 1-275)
Details on Acronym: [GM81]
[GM81]	(Gallagher+Mould, 1981)= (GM)
Write:	<<[GM81] NN>>
N:	12
Object:	Red Star (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=13, (Nos 0-12), No. 4 missing
in source:	NGC 205 = M 110
Ref:	=1981ApJ...244L...3G
by	GALLAGHER J.S. , MOULD J.R.
	Astrophys. J., 244, 3-6 (1981)
	Luminous red stars, in NGC 205.
o	<[GM81] NN> N=13, (Nos 0-12)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GM93]
[GM93]	(Gaylard+MacLeod, 1993)
Write:	<<[GM93] GLLL.ll+B.bb>>
N:	19
Object:	CH3OH Maser (SIMBAD class: Maser)
Note:	Hartebeeshoek radio observatory observations. See also [MG92].
Ref:	=1993MNRAS.262...43G
by	GAYLARD M.J. , MacLEOD G.C.
	Mon. Not. R. Astron. Soc., 262, 43-48 (1993)
	New detections of 6.6 GHz 5 1 -6 0 A+ methanol emission towards southern hydroxyl masers.
o	Table 1: <[GM93] GLLL.ll+B.bb> N=19.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GM98]
[GM98]	(Gal-Yam+Maoz, 1998)= ([GM98a])
Write:	<<[GM98] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=1 host galaxy of SN 1998CG
Ref:	=1998IAUC.6917Q...1G
by	GAL-YAM A. , MAOZ D., DAN J.
	IAU Circ., 6917, 1-None (1998)
	Supernova 1998cg in anonymous galaxy.
o	<[GM98] J121818.10+204430.0>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GM98a]
[GM98a]	(Gal-Yam+Maoz, 1998)
*****	Avoid the usage of [GM98a], prefer [GM98]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GM98b]
[GM98b]	(Guerrero+Manchado, 1998) (Not yet in Simbad)
Write:	<<[GM98b] Knot A>>
N:	4
Object:	Knot (SIMBAD class: Unknown = Object of Unknown Nature)
in source:	NGC 6881
Ref:	=1998ApJ...508..262G
by	GUERRERO M.A. , MANCHADO A.
	Astrophys. J., 508, 262-267 (1998)
	A precessing collimated outflow in the quadrupolar planetary nebula NGC 6881.
o	Fig.2: <[GM98b] Knot A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GM99]
[GM99]	(Gal-Yam+Maoz, 1999)= ([GM99a])
Write:	<<[GM99] JHHMMSS.ss+DDMMSS.s>>
N:	4
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	1999IAUC.7088Q...1G: host galaxy of SN 1999C. 1999IAUC.7181R...1G: host galaxies of SN 1999CG, SN 1999CH, SN 1999CI.
Ref:	=1999IAUC.7088Q...1G
by	GAL-YAM A. , MAOZ D.
	IAU Circ., 7088, 1-None (1999)
	Supernova 1999C in anonymous galaxy.
o	<[GM99] J100851.02+711042.9> N=1.
Ref:	=1999IAUC.7181R...1G
by	GAL-YAM A. , MAOZ D.
	IAU Circ., 7181, 1-None (1999)
	Supernovae 1999cg, 1999ch, 1999ci.
o	<[GM99] JHHMMSS.ss+DDMMSS.s> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GM99a]
[GM99a]	(Gal-Yam+Maoz, 1999)
*****	Avoid the usage of [GM99a], prefer [GM99]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GM99b]
[GM99b]	(Gyulbudaghian+May, 1999)
Write:	<<[GM99b] NN>> <<[GM99b] NN>>
N:	54+3
Object:	* + Globule (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 2: N=54 * in OB Assoc. Pup-CMa. p. 133: N=3 dark globules (Nos N1-N3).
in source:	NAME OB-Association Pup-CMa
Ref:	=1999Ap.....42..132G
by	GYULBUDAGHIAN A.L. , MAY J.
	Astrophysics, 42, 132-139 (1999)
	New OB-association in Pup-Cma.
o	Table 2: <[GM99b] NN> (Nos 1-54). Text: <[GM99b] AN> (Nos N1-N3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GMA
GMA	(Giant Molecular Assoc.)
*****	Avoid the usage of GMA, prefer [RK90]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GMA
GMA	(Giant Molecular Assoc.)
*****	Avoid the usage of GMA, prefer [TM97]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GMA2005]
[GMA2005]	(Goddi+Moscadelli+Alef+, 2005) (Not yet in Simbad)
Write:	<<[GMA2005] Sh 2-255 IR NN>> <<[GMA2005] IRAS 23139+5939 N>> <<[GMA2005] WB89 234 NN>> <<[GMA2005] OMC 2 N>>
N:	14+9+12+3
Object:	H2O Maser (SIMBAD class: Maser)
Note:	EVN observations of the 22.2GHz water masers features towards 4 high-mass star forming regions.
in source:	Sh 2-255:NAME Sh 2-255 IR = NAME Sh 2-255 IR
in source:	IRAS 23139+5939
in source:	WB89 234
in source:	OMC:OMC 2 = OMC 2
Ref:	=2005A&A...432..161G
by	GODDI C. , MOSCADELLI L., ALEF W., TARCHI A., BRAND J., PANI M.
	Astron. Astrophys., 432, 161-173 (2005)
	Kinematics of H_{2}O masers in high-mass star forming regions.
o	Table 3: <[GMA2005] Sh 2-255 IR NN> (Nos 1-14), <[GMA2005] IRAS 23139+5939 N> (Nos 1-9), <[GMA2005] WB89 234 NN> (Nos 1-12), <[GMA2005] OMC 2 N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMA98]
[GMA98]	(Gomez+Marscher+Alberdi+, 1998)
Write:	<<[GMA98] A>> <<[GMA98] a>> <<[GMA98] aN>> <<[GMA98] St>> <<[GMA98] Up>>
N:	17+14+2
Object:	Radio Jet (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio jets components of 3C 120 at 22 GHz 'A', radio jets components at 43 GHz, same letter, (but small letter) that at 22GHz (cross-id), and sub-components 'aN'. N=1 Stationary component: No. St. N=1 Extension component: No. Up.
in source:	3C 120
Ref:	=1998ApJ...499..221G
by	GOMEZ J. , MARSCHER A.P., ALBERDI A., MARTI J.M., IBANEZ J.M.
	Astrophys. J., 499, 221-226 (1998)
	Subparsec polarimetric radio observations of 3C 120: a close-up look at superluminal motion.
o	Table 1, Fig.1: <[GMA98] A> (Nos A-H) = <[GMA98] a> (Nos a-i), <[GMA98] aN> (Nos e1-e2, g1-g2), <[GMA98] St> N=1, <[GMA98] Up> N=1.
Ref:	=1999ApJ...521L..29G
by	GOMEZ J.-L. , MARSCHER A.P., ALBERDI A.
	Astrophys. J., 521, 29-32 (1999)
	86, 43, and 22 GHz VLBI observations of 3C 120.
o	Table 1, Fig.1: <[GMA98] A> (Nos I-N) = <[GMA98] a> (Nos i-n), <[GMA98] aN> (Nos f1-f2, i1-i2, k1-k2, n1-n2).
Ref:	=2000Sci...289.2317G
by	GOMEZ J.-L. , MARSCHER A.P., ALBERDI A., JORSTAD S.G., GARCIA-MIRO C.
	Science, 289, 2317-2320 (2000)
	Flashing superluminal components in the jet of the radio galaxy 3C 120.
o	<[GMA98] A> (No. O) added.
Ref:	=2001ApJ...561L.161G
by	GOMEZ J.-L. , MARSCHER A.P., ALBERDI A., JORSTAD S.G., AGUDO I.
	Astrophys. J., 561, 161-164 (2001)
	Monthly 43 GHz VLBA polarimetric monitoring of 3C 120 over 16 epochs: evidence for trailing shocks in a relativistic jet.
o	Fig.1: <[GMA98] aN> (Nos l2, s, r, o1, o2) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMA99]
[GMA99]	(Gal-Yam+Maoz+Anter, 1999)= ([GMA99a])
Write:	<<[GMA99] JHHMMSS.ss+DDMMSS.s>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Note:	N=3, host G of SN 1999CT, SN 1999CU and SN 1999CV
Ref:	=1999IAUC.7210R...1G
by	GAL-YAM A. , MAOZ D., ANTER A.
	IAU Circ., 7210, 1-None (1999)
	Supernovae 1999ct, 1999cu, 1999cv.
o	<[GMA99] JHHMMSS.ss+DDMMSS.s> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMA99a]
[GMA99a]	(Gal-Yam+Maoz+Anter, 1999)
*****	Avoid the usage of [GMA99a], prefer [GMA99]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMA99b]
[GMA99b]	(Gomez+Marscher+Alberdi+, 1999)
Write:	<<[GMA99b] 0735+178 A>> <<[GMA99b] 0735+178 aN>>
N:	9
Object:	(Rad) component (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio components of QSO 0735+178 Table 1, Fig.1: At 22GHz, (Nos A-C). Table 2, Fig.2: At 43GHz, (Nos a-d, b1-b2, c1-c3). Cross-id between the 2 formats. See also Gabuzda, [BZ91].
in source:	QSO B0735+178
Ref:	=1999ApJ...519..642G
by	GOMEZ J.-L. , MARSCHER A.P., ALBERDI A., GABUZDA D.C.
	Astrophys. J., 519, 642-646 (1999)
	The twisted parsec-scale structure of 0735+178.
o	Table 1, Fig.1: <[GMA99b] 0735+178 A> (Nos A-C). Table 2, Fig.2: <[GMA99b] 0735+178 aN> (Nos a-d, b1-b2, c1-c3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMA99c]
[GMA99c]	(Gomez+Marscher+Alberdi, 1999)
Write:	<<[GMA99c] Component St>> <<[GMA99c] Component A>> <<[GMA99c] Component w>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Structure of the QSO 3C 454.3. Component 'St' is the 'Stationary' component 1 in [PPZ87]. Component A is a new component. Component n is a faint component in the north direction. See also [PPZ87], [KDP96].
in source:	3C 454.3
Ref:	=1999ApJ...522...74G
by	GOMEZ J.-L. , MARSCHER A.P., ALBERDI A.
	Astrophys. J., 522, 74-81 (1999)
	Outburst in the polarized structure of the compact jet of 3C 454.3.
o	Core and Jet = [PPZ87] Core and Jet.
o	Table 2: <[GMA99c] Component St> N=1. <[GMA99c] Component A> N=1. <[GMA99c] Component n> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMA99d]
[GMA99d]	(Guainazzi+Matt+Antonelli+, 1999)
Write:	<<[GMA99d] N>>
N:	4
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations of Circinus galaxy field.
Ref:	=1999MNRAS.310...10G
by	GUAINAZZI M. , MATT G., ANTONELLI L.A., BASSANI L., FABIAN A.C., MAIOLINO R., MARCONI A., FIORE F., IWASAWA K., PIRO L.
	Mon. Not. R. Astron. Soc., 310, 10-20 (1999)
	Soft X-ray spectroscopy of Compton-thick Seyfert 2 galaxies with BeppoSAX.
o	Table 6: <[GMA99d] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GMASS
GMASS	(Galaxy Mass Assembly Spectroscopic Survey)
Write:	<<GMASS NNNN>>
Object:	G (SIMBAD class: Galaxy)
Note:	Galaxy Mass Assembly ultradeep Spectroscopic Survey. VLT FORS2 spectroscopy of 4.5mu.m (Spitzer) selected galaxies from the GOODS-South field.
Ref:	=2008A&A...482...21C
by	CIMATTI A. , CASSATA P., POZZETTI L., KURK J., MIGNOLI M., RENZINI A., DADDI E., BOLZONELLA M., BRUSA M., RODIGHIERO G., DICKINSON M., FRANCESCHINI A., ZAMORANI G., BERTA S., ROSATI P., HALLIDAY C.
	Astron. Astrophys., 482, 21-42 (2008)
	GMASS ultradeep spectroscopy of galaxies at z ~ 2. II. Superdense passive galaxies: how did they form and evolve?
o	Table 1: <GMASS NNNN> N=13 among (Nos 472-2559).
Ref:	=2009A&A...504..331K
by	KURK J. , CIMATTI A., ZAMORANI G., HALLIDAY C., MIGNOLI M., POZZETTI L., DADDI E., ROSATI P., DICKINSON M., BOLZONELLA M., CASSATA P., RENZINI A., FRANCESCHINI A., RODIGHIERO G., BERTA S.
	Astron. Astrophys., 504, 331-346 (2009)
	GMASS ultradeep spectroscopy of galaxies at z ~ 2. V. Witnessing the assembly at z = 1.6 of a galaxy cluster.
o	Table 1: <GMASS NNNN> N=42 among (Nos 365-2603).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Gmb
Gmb	(Groombridge)= (Gr) = (Grb) = Groombridge
Write:	<<Gmb NNNN>>
N:	4243
Object:	* (SIMBAD class: Star)
Ref:	=1905Gmb...C......0D
by	DYSON F.W. , THACKERAY W.G., CHRISTIE W.H.M.
	Proceeding of the Royal Soc., Edinburgh, 0-None (1905)
	New reduction of Groombridge's catalogue of circumpolar stars.
o	<Gmb NNNN> (Nos 1-4243).
Details on Acronym: [GMB2000]
[GMB2000]	(Guainazzi+Matt+Brandt+, 2000)
Write:	<<[GMB2000] SN>> <<[GMB2000] N>>
N:	2+4
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Figs 1, 3: N=2 BeppoSAX serendipitous sources, (Nos S1-S2) in the field of NGC 4945. Table 1, Fig.3: N=4 ROSAT PSPC sources (Nos 1-4) in NGC 4945.
in source:	NGC 4945
Ref:	=2000A&A...356..463G
by	GUAINAZZI M. , MATT G., BRANDT W.N., ANTONELLI L.A., BARR P., BASSANI L.
	Astron. Astrophys., 356, 463-474 (2000)
	A broad-band X-ray view of NGC 4945.
o	Figs 1, 3: <[GMB2000] SN> (Nos S1-S2). Table 1, Fig.3: <[GMB2000] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMB2007]
[GMB2007]	(Gil de Paz+Madore+Boissier+, 2007)= ([GMB2007a])
Write:	<<[GMB2007] NGC 5236 XUV NN>> <<[GMB2007] NGC 4625 XUV NN>> <<[GMB2007] Background G N>>
N:	22+12+2
Object:	(UV) + G (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	GALEX photometry and 6.5m Magellan-I telescope IMACS and Palomar Observatory 5m Hale telescope COSMIC spectroscopy of the fields of of M83 (NGC 5236) and NGC 4625.
in source:	NGC 4625
in source:	NGC 5236
Ref:	=2007ApJ...661..115G
by	GIL DE PAZ A. , MADORE B.F., BOISSIER S., THILKER D., BIANCHI L., SANCHEZ CONTRERAS C., BARLOW T.A., CONROW T., FORSTER K., FRIEDMAN P.G., MARTIN D.C., MORRISSEY P., NEFF S.G., RICH R.M., SCHIMINOVICH D., SEIBERT M., SMALL T., DONAS J., HECKMAN T.M., LEE Y.-W., MILLIARD B., SZALAY A.S., WYDER T.K., YI S.
	Astrophys. J., 661, 115-134 (2007)
	Chemical and photometric evolution of extended ultraviolet disks: optical spectroscopy of M83 (NGC 5236) and NGC 4625.
o	Table 2: <[GMB2007] NGC 5236 XUV NN> (Nos 1-22), <[GMB2007] NGC 4625 XUV NN> (Nos 1-12). text: <[GMB2007] Background G N> (Nos 1-2).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GMB2007a]
[GMB2007a]	(Gil de Paz+Madore+Boissier+, 2007)
*****	Avoid the usage of [GMB2007a], prefer [GMB2007]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMB2007b]
[GMB2007b]	(Garay+Mardones+Brooks+, 2007)
Write:	<<[GMB2007b] JHHMMSS.s+DDMMSS>> <<[GMB2007b] HHMMm+DDMM A>> <<[GMB2007b] HHMMm+DDMM halo>> <<[GMB2007b] HHMMm+DDMM core>> <<[GMB2007b] HHMMm+DDMM filament>>
N:	20+16
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	SEST SIMBA 1.2mm observations of 18 IRAS HII starforming regions.
Ref:	=2007ApJ...666..309G
by	GARAY G. , MARDONES D., BROOKS K.J., VIDELA L., CONTRERAS Y.
	Astrophys. J., 666, 309-320 (2007)
	A multiwavelength study of young massive star forming regions. II. The dust environment.
o	Table 2: <[GMB2007b] JHHMMSS.s+DDMMSS> N=20. Table 3: <[GMB2007b] HHMMm+DDMM A>, <[GMB2007b] HHMMm+DDMM halo>, <[GMB2007b] HHMMm+DDMM core>, <[GMB2007b] HHMMm+DDMM filament> N=16.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMB2010]
[GMB2010]	(Geller+Mathieu+Braden+, 2010)= (WOCS) = ([GMB2010a])
Write:	<<[GMB2010] WOCS NNNFFF>>
N:	1151
Object:	* (SIMBAD class: Star)
Note:	Radial velocity measurements in M35 from the WIYN Open Cluster Study (WOCS). The identification number is the three digit star number followed by the three digit annulus number. See also [HGM2009b].
in source:	NGC 2168
Ref:	=2010AJ....139.1383G
by	GELLER A.M. , MATHIEU R.D., BRADEN E.K., MEIBOM S., PLATAIS I., DOLAN C.J.
	Astron. J., 139, 1383-1393 (2010)
	WIYN open cluster study. XXXVIII. Stellar radial velocities in the young open cluster M35 (NGC 2168).
o	Table 1: <[GMB2010] WOCS NNNFFF> N=1151.
=E=	Catalogue in electronic form as <J/AJ/139/1383/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMB2010a]
[GMB2010a]	(Geller+Mathieu+Braden+, 2010)= (WOCS)
Note:	Radial velocity measurements in M35 from the WIYN Open Cluster Study (WOCS).
*****	Avoid the usage of [GMB2010a], prefer [GMB2010]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMB2010b]
[GMB2010b]	(Garay+Mardones+Bronfman+, 2010)
Write:	<<[GMB2010b] GLLL.lll+B.bbbA>>
N:	5
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	SEST SIMBA 1.2mm continuum observations of a star-forming region in the Norma Spiral arm.
Ref:	=2010ApJ...710..567G
by	GARAY G. , MARDONES D., BRONFMAN L., MAY J., CHAVARRIA L., NYMAN L.-A.
	Astrophys. J., 710, 567-582 (2010)
	Four highly luminous massive star-forming regions in the Norma spiral arm. I. Molecular gas and dust observations.
o	Tables 6-7: <[GMB2010b] GLLL.lll+B.bbbA> N=5
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMB2010c]
[GMB2010c]	(Green+Myers+Barkhouse+, 2010)
Write:	<<[GMB2010c] SDSS J1254+0846>>
N:	1
Object:	Binary quasar (SIMBAD class: InteractingG = Interacting Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Magellan Baade telescope IMACS (optical spectroscopy and imaging), Chandra ACIS X-ray, VLA (8.5GHz) observations of N=1 binary quasar.
Ref:	=2010ApJ...710.1578G
by	GREEN P.J. , MYERS A.D., BARKHOUSE W.A., MULCHAEY J.S., BENNERT V.N., COX T.J., ALDCROFT T.L.
	Astrophys. J., 710, 1578-1588 (2010)
	SDSS J1254+0846: a binary quasar caught in the act of merging.
o	SDSS J153636.22+1044127.0 is a misprint for SDSS J153636.22+044127.0.
o	<[GMB2010c] SDSS J1254+0846> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMB2011]
[GMB2011]	(Geach+Murphy+Bower, 2011)
Write:	<<[GMB2011] NNNN>>
N:	4098
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=4098 photometrically selected galaxy clusters with a median redshift z=0.32 in the 'Stripe 82' region of the Sloan Digital Sky Survey (SDSS).
Ref:	=2011MNRAS.413.3059G
by	GEACH J.E. , MURPHY D.N.A., BOWER R.G.
	Mon. Not. R. Astron. Soc., 413, 3059-3067 (2011)
	4098 galaxy clusters to z~ 0.6 in the Sloan digital sky survey equatorial stripe 82.
o	clusters.dat: <[GMB2011] NNNN> (Nos 1-4098).
=E=	Catalogue in electronic form as J/MNRAS/413/3059
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMB2015]
[GMB2015]	(Girardi+Mercurio+Balestra+, 2015)
Write:	<<[GMB2015] NNN>>
N:	412
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT VIMOS and FORS2 spectroscopic observations of N=412 galaxies in the massive galaxy cluster MACS J1206.2-0847.
in source:	MCS J1206.2-0847
Ref:	=2015A&A...579A...4G
by	GIRARDI M. , MERCURIO A., BALESTRA I., NONINO M., BIVIANO A., GRILLO C., ROSATI P., ANNUNZIATELLA M., DEMARCO R., FRITZ A., GOBAT R., LEMZE D., PRESOTTO V., SCODEGGIO M., TOZZI P., BARTOSCH CAMINHA G., BRESCIA M., COE D., KELSON D., KOEKEMOER A., LOMBARDI M., MEDEZINSKI E., POSTMAN M., SARTORIS B., UMETSU K., ZITRIN A., BOSCHIN W., CZOSKE O., DE LUCIA G., KUCHNER U., MAIER C., MENEGHETTI M., MONACO P., MONNA A., MUNARI E., SEITZ S., VERDUGO M., ZIEGLER B.
	Astron. Astrophys., 579A, 4-4 (2015)
	CLASH-VLT: Substructure in the galaxy cluster MACS J1206.2-0847 from kinematics of galaxy populations.
o	Table 2: <[GMB2015] NNN> N=412.
=E=	Catalogue in electronic form as J/A+A/579/A4
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GMBCG
GMBCG	(Gaussian Mixture Brightest Cluster Galaxy)
Write:	<<GMBCG DDD.ddddd+DD.ddddd>> <<GMBCG JDDD.ddddd+DD.ddddd>> (not recognised by Simbad, but found in literature)
N:	55424
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	Catalog of N=55424 optically selected galaxy clusters from the application of a new Gaussian Mixture Brightest Cluster Galaxy (GMBCG) algorithm to SDSS DR7 data. More information available at: http://home.fnal.gov/~jghao/gmbcg_sdss_catalog.html
Ref:	=2010ApJS..191..254H
by	HAO J. , McKAY T.A., KOESTER B.P., RYKOFF E.S., ROZO E., ANNIS J., WECHSLER R.H., EVRARD A., SIEGEL S.R., BECKER M., BUSHA M., GERDES D., JOHNSTON D.E., SHELDON E.
	Astrophys. J., Suppl. Ser., 191, 254-274 (2010)
	A GMBCG galaxy cluster catalog of 55,424 rich clusters from SDSS DR7.
o	<GMBCG DDD.ddddd+DD.ddddd> N=55424.
=E=	Catalogue in electronic form as <J/ApJS/191/254/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GMC
GMC	(Giant Molecular Cloud)
*****	Avoid the usage of GMC, prefer [DRG92]
Origin	of the Acronym: L (2001ApJ...551..687M)
Details on Acronym: GMC
GMC	(Gratier+Braine+Rodriguez-Fernandez+, 2010)
*****	Avoid the usage of GMC, prefer [GBR2010]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GMC
GMC	(Giant Molecular Cloud)
*****	Avoid the usage of GMC, prefer [GCB88]
Origin	of the Acronym: L (2000A&A...357..308G)
Details on Acronym: GMC
GMC	(Galera-Rosillo+Corradi+Mampaso)
*****	Avoid the usage of GMC, prefer [GCM2018]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GMC
GMC	(Giant Molecular Cloud)
*****	Avoid the usage of GMC, prefer [MTB2001]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GMC
GMC	(Giant Molecular Cloud)
*****	Avoid the usage of GMC, prefer [THK99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GMC2001]
[GMC2001]	(Glass+Matsumoto+Carter+, 2001)= (GMCS)
Write:	<<[GMC2001] FF-NNNN>>
N:	399
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Study of Long Period Variables stars near the Galactic Center. In the format FF stands for the subfield number (Nos 1-25), NNNN is a DOPHOT running number. N=411, but 12 are the same observed in 2 overlapping fields.
in source:	NAME Gal Center
Ref:	=2001MNRAS.321...77G
by	GLASS I.S. , MATSUMOTO S., CARTER B.S., SEKIGUCHI K.
	Mon. Not. R. Astron. Soc., 321, 77-95 (2001)
	Large-amplitude variables near the Galactic Centre.
o	(Erratum) erratum vol. 336, p. 1390 (2002)
o	Tables 2, 4: <[GMC2001] FF-NNNN> N=399.
=E=	Catalogue in electronic form as J/MNRAS/321/77
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMC2003]
[GMC2003]	(Ganguly+Masiero+Charlton+, 2003)
Write:	<<[GMC2003] RX J1230.8+0115 A>> <<[GMC2003] QSO J1230+0115 abs N.NNNN>> <<[GMC2003] RX J1230.8+0115 AN>> <<[GMC2003] QSO J1230+0115 abs N.NNNNN>>
N:	4+11
Object:	Absorber
Stat:	is completely incorporated in Simbad
Note:	HST and FUSE spectra of the RX J1230.8+0115 = QSO J1230+0115. N=4 absorption systems with 11 components.
Ref:	=2003ApJ...598..922G
by	GANGULY R. , MASIERO J., CHARLTON J.C., SEMBACH K.R.
	Astrophys. J., 598, 922-934 (2003)
	An intrinsic absorption complex toward RX J1230.8+0115: geometry and photoionization conditions.
o	Text: <[GMC2003] RX J1230.8+0115 A> (Nos A-D) = <[GMC2003] QSO J1230+0115 abs N.NNNN> N=4. Table 1: <[GMC2003] RX J1230.8+0115 AN> (Nos A1, B1-B3, C1-C2, D1-D5) = <[GMC2003] QSO J1230+0115 abs N.NNNNN> N=11.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMC2004]
[GMC2004]	(Giannini+McCoey+Caratti o Garatti+, 2004)= ([GMC2004a])
Write:	<<[GMC2004] N>>
N:	9
Object:	Outflow (SIMBAD class: Outflow)
Note:	ESO NTT SOFI long slit spectroscopy of N=9 H2 emission knots in BHR 71. See also [B2001b].
in source:	BHR 71
Ref:	=2004A&A...419..999G
by	GIANNINI T. , McCOEY C., CARATTI O GARATTI A., NISINI B., LORENZETTI D., FLOWER D.R.
	Astron. Astrophys., 419, 999-1014 (2004)
	On the excitation of the infrared knots along protostellar jets.
o	Fig.3: <[GMC2004] N> (Nos 1-9).
=E=	Catalogue in electronic form as J/A+A/419/999
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMC2004a]
[GMC2004a]	(Giannini+McCoey+Caratti o Garatti+, 2004)
*****	Avoid the usage of [GMC2004a], prefer [GMC2004]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMC2004b]
[GMC2004b]	(Goncalves+Mampaso+Corradi+, 2004) (Not yet in Simbad)
Write:	<<[GMC2004b] K 4-47 Knot N>> <<[GMC2004b] K 4-47 Core>>
N:	2+1
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	PN K 4-47 is an unusual PN composed of a compact core and a pair of low-ionization knots.
in source:	PN K 4-47
Ref:	=2004MNRAS.355...37G
by	GONCALVES D.R. , MAMPASO A., CORRADI R.L.M., PERINOTTO M., RIERA A., LOPEZ-MARTIN L.
	Mon. Not. R. Astron. Soc., 355, 37-43 (2004)
	K 4-47: a planetary nebula excited by photons and shocks.
o	Fig.1: <[GMC2004b] K 4-47 Knot N> (Nos 1-2), <[GMC2004b] K 4-47 Core> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMC2010]
[GMC2010]	(Greissl+Meyer+Christopher+, 2010)
Write:	<<[GMC2010] Cluster 89/90>>
N:	1
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	Keck NIRSPEC observations of N=1 massive star cluster in the overlap region of the Antennae (NGC 4038/39).
in source:	NAME THE ANTENNAE = NAME NGC 4038 9
Ref:	=2010ApJ...710.1746G
by	GREISSL J. , MEYER M.R., CHRISTOPHER M.H., SCOVILLE N.Z.
	Astrophys. J., 710, 1746-1754 (2010)
	Star formation history of a young super-star cluster in NGC 4038/39: direct detection of low-mass pre-main sequence stars.
o	<[GMC2010] Cluster 89/90> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMC98]
[GMC98]	(Gregorio-Hetem+Montmerle+Casanova+, 1998)= (GMCF)
Write:	<<[GMC98] Mon X-NN>> <<[GMC98] Rosette X-NN>> <<[GMC98] Rosette IR-N>>
N:	48+29+7
Object:	(X) + (IR) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT observations. Table 2a, 2b: N=48 X-ray sources in Monoceros field, (Nos 1-41) are ROSAT sources detected, (Nos 42-48) are additional possible X-ray sources. Table 3a, 3b: N=29 X-ray sources in Rosette field, (Nos 1-21) are ROSAT sources detected, (Nos 22-29) are additional possible X-ray sources. Table 6: N=7 Rosette IR-clusters possibly associated with X-ray emission. See also [CMD97]
in source:	NAME Mon R2 GMC
in source:	NAME Rosette Molecular Cloud
Ref:	=1998A&A...331..193G
by	GREGORIO-HETEM J. , MONTMERLE T., CASANOVA S., FEIGELSON E.D.
	Astron. Astrophys., 331, 193-210 (1998)
	X-rays and star formation: ROSAT observations of the Monoceros and Rosette molecular clouds.
o	Table 5: IRNNN = [CMD97] NNN
o	Table 2a, 2b: <[GMC98] Mon X-NN> (Nos 1-48). Table 3a, 3b: <[GMC98] Rosette X-NN> (Nos 1-29). Table 6: <[GMC98] Rosette IR-N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMC99]
[GMC99]	(Glass+Matsumoto+Carter+, 1999)= ([GMC99a])
Write:	<<[GMC99] DNNNN>>
N:	19
Object:	* in Cl* (SIMBAD class: Star)
Note:	N=19 stars, probable members of the Quintuplet cluster. The format 'DNNNN' is a DOPHOT running number.
in source:	NAME Quintuplet Cluster
Ref:	=1999MNRAS.304L..10G
by	GLASS I.S. , MATSUMOTO S., CARTER B.S., SEKIGUCHI K.
	Mon. Not. R. Astron. Soc., 304, 10-14 (1999)
	Luminous variables in the Quintuplet cluster.
o	Table 1: Q1 to Q15 = GMM 1 to 15, (NNN) = qF NNN.
o	Table 1: <[GMC99] DNNNN> N=19 among (Nos D4 to D3606).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMC99a]
[GMC99a]	(Glass+Matsumoto+Carter+, 1999)
*****	Avoid the usage of [GMC99a], prefer [GMC99]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMC99b]
[GMC99b]	(Georgakakis+Mobasher+Cram+, 1999)= (Phoenix-Deep)
Write:	<<[GMC99b] NNN>>
N:	246
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA radio survey. The classification is based on optic spectroscopy. Positions are based on optical imaging. Catalogue of N=246 faint radio-sources.
Ref:	=1999MNRAS.306..708G
by	GEORGAKAKIS A. , MOBASHER B., CRAM L., HOPKINS A., LIDMAN C., ROWAN-ROBINSON M.
	Mon. Not. R. Astron. Soc., 306, 708-726 (1999)
	The Phoenix Survey: optical and near-infrared observations of faint radio sources.
o	Table 1: <[GMC99b] NNN> (Nos 1-246).
=E=	Catalogue in electronic form as J/MNRAS/306/708
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GMCF
GMCF	(Gregorio-Hetem+Montmerle+Casanova+Feigelson)
*****	Avoid the usage of GMCF, prefer [GMC98]
Origin	of the Acronym: L (2003PASJ...55..635N)
Details on Acronym: GMCS
GMCS	(Glass+Matsumoto+Carter+Sekiguchi)
*****	Avoid the usage of GMCS, prefer [GMC2001]
Origin	of the Acronym: L (2004PASJ...56..261D)
Details on Acronym: [GMD93]
[GMD93]	(Gizis+Mould+Djorgovski, 1993)
Write:	<<[GMD93] NN>>
N:	19
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations
in source:	NAME Fornax Dwarf Galaxy
Ref:	=1993PASP..105..871G
by	GIZIS J.E. , MOULD J.R., DJORGOVSKI S.
	Publ. Astron. Soc. Pac., 105, 871-874 (1993)
	An X-ray image of the Fornax dwarf spheroidal galaxy.
o	Table 1: <[GMD93] NN> N=19
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMD97]
[GMD97]	(Gunn+Migenes+Doyle+, 1997)
Write:	<<[GMD97] JHHMMSS+DDMMSS>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATNF observations. N=3 radio-sources in the field of CF Tuc. See also [BJS99]
Ref:	=1997MNRAS.287..199G
by	GUNN A.G. , MIGENES V., DOYLE J.G., SPENCER R.E., MATHIOUDAKIS M.
	Mon. Not. R. Astron. Soc., 287, 199-210 (1997)
	Radio and extreme-ultraviolet observations of CF Tucanae.
o	text, p.203: <[GMD97] JHHMMSS+DDMMSS> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMD98]
[GMD98]	(Gal-Yam+Maoz+Dan+, 1998)
Write:	<<[GMD98] JHHMMSS.ss+DDMMSS.s>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Wise Observatory Optical Transients Search (WOOTS). N=2 host galaxies of SNr.
Ref:	=1998IAUC.7055Q...1G
by	GAL-YAM A. , MAOZ D., DAN J., IBBETSON P.
	IAU Circ., 7055, 1-None (1998)
	Supernovae 1998eu and 1998ev in anonymous galaxies.
o	<[GMD98] J005958.66+141800.4>, <[GMD98] J010412.68+250059.1>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMD99]
[GMD99]	(Gal-Yam+Maoz+Dan+, 1999)
Write:	<<[GMD99] JHHMMSS.ss+DDMMSS.s>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=2 host galaxies of SN 1998FC (J025914.01+032955.7) and SN 1998FD (J011917.66+155521.3).
Ref:	=1999IAUC.7082Q...1G
by	GAL-YAM A. , MAOZ D., DAN J., BEERI R.
	IAU Circ., 7082, 1-None (1999)
	Supernovae 1998fc and 1998fd in anonymous galaxies.
o	<[GMD99] JHHMMSS.ss+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GME93]
[GME93]	(Gomez de Castro+Miranda+Eiroa, 1993)
Write:	<<[GME93] GGD 34 A>>
N:	3+7
Object:	Condensation (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=3 condensations in GGD 34 (Nos A-C), See also [GR99].
in source:	GGD 34
Ref:	=1993A&A...267..559G
by	GOMEZ DE CASTRO A.I. , MIRANDA L.F., EIROA C.
	Astron. Astrophys., 267, 559-566 (1993)
	A kinematical study of the jet GGD 34.
o	<[GME93] GGD 34 A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMF2004]
[GMF2004]	(Gavazzi+Mellier+Fort+, 2004)
Write:	<<[GMF2004] DD.dddd+DD.dddd>>
N:	96508
Object:	G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	CFHT observations with the CFH12K camera of the supercluster ClG 0302+1717. Identification of stars, foreground and background early type galaxies. Photometric and weak lensing analysis of the galaxy sample.
in source:	ClG 0302+1717
Ref:	=2004A&A...422..407G
by	GAVAZZI R. , MELLIER Y., FORT B., CUILLANDRE J.-C., DANTEL-FORT M.
	Astron. Astrophys., 422, 407-422 (2004)
	Mass and light in the supercluster of galaxies MS0302+17.
o	Objects of the catalog not in Simbad.
o	Catalog: <[GMF2004] DD.dddd+DD.dddd> N=96508.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMF2005]
[GMF2005]	(Govoni+Murgia+Feretti+, 2005)
Write:	<<[GMF2005] AN>>
N:	5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 1.4GHz observations of the A2255 cluster of galaxies, showing a relic R, a bridge B, and three straight filaments F1, F2, F3.
in source:	ACO 2255
Ref:	=2005A&A...430L...5G
by	GOVONI F. , MURGIA M., FERETTI L., GIOVANNINI G., DALLACASA D., TAYLOR G.B.
	Astron. Astrophys., 430, 5-8 (2005)
	A2255: The first detection of filamentary polarized emission in a radio halo.
o	Fig. 1: <[GMF2005] AN> (Nos B, R, F1-F3).
o	1E0657-57 = 1ES 0657-55.8 in SIMBAD
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMF2013]
[GMF2013]	(Gezari+Martin+Forster+, 2013)
Write:	<<[GMF2013] XMMLSS MOSNN-NN>> <<[GMF2013] CDFS MOSNN-NN>> <<[GMF2013] COSMOS MOSNN-NN>> <<[GMF2013] GROTH MOSNN-NN>> <<[GMF2013] ELAISN1 MOSNN-NN>> <<[GMF2013] VVDS22H MOSNN-NN>> <<[GMF2013] XMMLSS_MOSNN-NN>> (not recognised by Simbad, but found in literature) <<[GMF2013] CDFS_MOSNN-NN>> <<[GMF2013] COSMOS_MOSNN-NN>> <<[GMF2013] GROTH_MOSNN-NN>> <<[GMF2013] ELAISN1_MOSNN-NN>> <<[GMF2013] VVDS22H_MOSNN-NN>>
N:	1078
Object:	UV Variable Source (SIMBAD class: UV = UV-emission Source)
Note:	N=1078 ultraviolet (UV) variable sources discovered in ∼40 sq. degrees of GALEX Time Domain Survey (TDS) NUV images. The GALEX TDS fields were designed to be in spatial and temporal coordination with the Pan-STARRS1 Medium Deep Survey. The formats are based on the field name followed by the MOS pointing number. Use of Pan-STARRS1 Medium Deep Survey (PS1 MDS) data.
Ref:	=2013ApJ...766...60G
by	GEZARI S. , MARTIN D.C., FORSTER K., NEILL J.D., HUBER M., HECKMAN T., BIANCHI L., MORRISSEY P., NEFF S.G., SEIBERT M., SCHIMINOVICH D., WYDER T.K., BURGETT W.S., CHAMBERS K.C., KAISER N., MAGNIER E.A., PRICE P.A., TONRY J.L.
	Astrophys. J., 766, 60 (2013)
	The GALEX Time Domain Survey. I. Selection and classification of over a thousand ultraviolet variable sources.
o	Table 4: <[GMF2013] XMMLSS MOSNN NN> N=169, <[GMF2013] CDFS MOSNN NN> N=247, <[GMF2013] COSMOS MOSNN NN> N=199, <[GMF2013] GROTH MOSNN NN> N=177, <[GMF2013] ELAISN1 MOSNN NN> N=160, <[GMF2013] VVDS22H MOSNN NN> N=126.
=E=	Catalogue in electronic form as <J/ApJ/766/60/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMF2016]
[GMF2016]	(Gong+Mao+Fang+, 2016)
Write:	<<[GMF2016] NN km s-1 cloud>> <<[GMF2016] Shell A>> <<[GMF2016] Shell-MonOB3>> <<[GMF2016] A>> <<[GMF2016] DNN>> <<[GMF2016] JHHMMSS.ss+DDMMSS.s>>
N:	3+3+1+7+15+163
Object:	MCld + Shell + Clump + Dust Clump + Poss. YSO (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Purple Mountain Observatory (PMO) 13.7m telescope 3x3-beam Superconducting Spectroscopic Array Receiver (SSAR) observations toward the Galactic Plane of N=3 molecular clouds, N=1+3 molecular shells, N=7 C18O clumps, N=15 dust clumps, and N=163 YSO candidates. Use of BGPS, 2MASS, and WISE archival data.
Ref:	=2016A&A...588A.104G
by	GONG Y. , MAO R.Q., FANG M., ZHANG S.B., SU Y., YANG J., JIANG Z.B., XU Y., WANG M., WANG Y., LU D.R., SUN J.X.
	Astron. Astrophys., 588A, 104-104 (2016)
	Molecular clouds and star formation toward the Galactic plane within 216.25° ≤ l ≤ 218.75° and -0.75° ≤ b ≤ 1.25°.
o	Fig. 2, Table 1: <[GMF2016] NN km s-1 cloud> (Nos 15, 27, 50). Fig. 3, Table 3: <[GMF2016] Shell A> (Nos A-C). Fig. 5, Table 3: <[GMF2016] Shell-MonOB3> N=1. Figs 10-11, Table 4: <[GMF2016] A> (Nos A-G). Table 6: <[GMF2016] DNN> (Nos D1-D15). Table D.1: <[GMF2016] JHHMMSS.ss+DDMMSS.s> N=163.
=E=	Catalogue in electronic form as <J/A+A/588/A104/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMF97]
[GMF97]	(Grosso+Montmerle+Feigelson+, 1997) (Not yet in Simbad)
Write:	<<[GMF97] NN>>
N:	13
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT HRI observations
in source:	NAME rho Oph Cloud
Ref:	=1997Natur.387...56G
by	GROSSO N. , MONTMERLE T., FEIGELSON E.D., ANDRE P., CASANOVA S., GREGORIO-HETEM J.
	Nature, 387, 56-58 (1997)
	An X-ray superflare from an infrared protostar.
o	Fig.1: <[GMG97] NN> N=5 among 13
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMG2001]
[GMG2001]	(Garrett+Muxlow+Garrington+, 2001)= (VLA)
Write:	<<[GMG2001] VLA JHHMMSS+DDMMSS>> <<[GMG2001] VLA JHHMMSS+DDMMSS a>>
N:	3+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	observations of HDF. Detection of 3 VLA sources. One of the source 'VLA J123644+621133' has a compact core component 'c' and an additional component 'j'.
in source:	NAME HDFN
Ref:	=2001A&A...366L...5G
by	GARRETT M.A. , MUXLOW T.W.B., GARRINGTON S.T., ALEF W., ALBERDI A., VAN LANGEVELDE H.J., VENTURI T., POLATIDIS A.G., KELLERMANN K.I., BAAN W.A., KUS A., WILKINSON P.N., RICHARDS A.M.S.
	Astron. Astrophys., 366, 5-8 (2001)
	AGN and starbursts at high redshift: High resolution EVN radio observations of the Hubble Deep Field.
o	Table 1: <[GMG2001] VLA JHHMMSS+DDMMSS> N=3, <[GMG2001] VLA J123644+621133 a> (Nos c, j).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMG2003]
[GMG2003]	(Gal-Yam+Maoz+Guhathakurta+, 2003)
Write:	<<[GMG2003] SN 1998FC Galaxy N>> <<[GMG2003] SN 2001AL Galaxy N>> <<[GMG2003] SN 2001AL Source N>>
N:	1+2+3
Object:	G + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Galaxies and sources observed in the field of SN 1998FC and SN 2001AL, discovered in the WOOTS survey.
Ref:	=2003AJ....125.1087G
by	GAL-YAM A. , MAOZ D., GUHATHAKURTA P., FILIPPENKO A.V.
	Astron. J., 125, 1087-1094 (2003)
	A population of intergalactic supernovae in galaxy clusters.
o	Fig.1: <[GMG2003] SN 1998FC Galaxy N> (No. 1). Fig.2: <[GMG2003] SN 2001AL Galaxy N> (Nos 1-2), <[GMG2003] SN 2001AL Source N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMG2004]
[GMG2004]	(Gyulbudaghian+May+Gonzalez+, 2004)= (SNO)
Write:	<<[GMG2004] NN>>
N:	93
Object:	Nebula (SIMBAD class: ISM = Interstellar Medium Object)
Note:	The authors inspected plates of the Southern Hemisphere and find previously unreported nebulous objects.
Ref:	=2004RMxAA..40..137G
by	GYULBUDAGHIAN A.L. , MAY J., GONZALEZ L., MENDEZ R.A.
	Rev. Mex. Astron. Astrofis., 40, 137-146 (2004)
	Nebulous objects in the Southern Hemisphere.
o	Several errors in Table 1 reported by B. Skiff
o	Table 1: <[GMG2004] NN> (Nos 1-93).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMG2011]
[GMG2011]	(Govoni+Murgia+Giovannini+, 2011)
Write:	<<[GMG2011] A>>
N:	11
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	N=11 discrete radio sources in Abell 781. Use of archival VLA observations at 1400 and 325MHz.
in source:	ACO 781
Ref:	=2011A&A...529A..69G
by	GOVONI F. , MURGIA M., GIOVANNINI G., VACCA V., BONAFEDE A.
	Astron. Astrophys., 529A, 69-69 (2011)
	The large-scale diffuse radio emission in A781.
o	Figs 2+4, Table 2: <[GMG2011] A> (Nos A-L), No. K missing.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMG2015]
[GMG2015]	(Giallongo+Menci+Grazian+, 2015)
Write:	<<[GMG2015] A>>
N:	11
Object:	LSB Dwarf G (SIMBAD class: LowSurfBrghtG = Low Surface Brightness Galaxy)
Stat:	is completely incorporated in Simbad
Note:	LBT LBC deep observation of N=11 low surface brightness (LSB) dwarf galaxies in the Virgo Cluster.
in source:	NAME Virgo Cluster
Ref:	=2015ApJ...813...68G
by	GIALLONGO E. , MENCI N., GRAZIAN A., FASSBENDER R., FONTANA A., PARIS D., PENTERICCI L.
	Astrophys. J., 813, 68 (2015)
	The detection of ultra-faint low surface brightness dwarf galaxies in the Virgo cluster: a probe of dark matter and baryonic physics.
o	Table 1: <[GMG2015] A> (Nos A-L).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMG83]
[GMG83]	(Griffiths+Murray+Giacconi+, 1983)= (Pavo)
Write:	<<[GMG83] NN>>
N:	17
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Einstein X-ray survey
Ref:	=1983ApJ...269..375G
by	GRIFFITHS R.E. , MURRAY S.S., GIACCONI R., BECHTOLD J., MURDIN P., SMITH M., MacGILLIVRAY H.T., WARD M., DANZIGER J., LUB J., PETERSON B.A., WRIGHT A.E., BATTY M.J., JAUNCEY D.L., MALIN D.F.
	Astrophys. J., 269, 375-386 (1983)
	The optical identification content of the Einstein Observatory deep survey of a region in Pavo.
o	Table 1: <[GMG83] NN> (Nos 1-17)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMG98]
[GMG98]	(Gaensler+Manchester+Green, 1998)
Write:	<<[GMG98] N>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=4 radio-sources in the vicinity of SNR 296.8-00.3
in source:	NAME HDFN
Ref:	=1998MNRAS.296..813G
by	GAENSLER B.M. , MANCHESTER R.N., GREEN A.J.
	Mon. Not. R. Astron. Soc., 296, 813-823 (1998)
	Radio continuum and H I observations of the supernova remnant G296.8-00.3.
o	Strip, rim, and other structures shown on the Figures are not in SIMBAD.
o	Table 4: <[GMG98] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMH2020]
[GMH2020]	(Ge+Mardones+He+, 2020)
Write:	<<[GMH2020] CN>>
N:	4
Object:	Core (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	JCMT SCUBA2 850µm and Nobeyama 45m telescope N2H+, HC3N, and CCS observations of N=4 cores in the Planck Galactic cold clump PLCKECC G224.47-00.65.
Ref:	=2020ApJ...891...36G
by	GE J.X. , MARDONES D., HE J.H., RAWLINGS J.M.C., LIU S.-Y., LEE J.-E., TATEMATSU K., LIU T., ZHU L., CHANG Q., INOSTROZA N., FENG S.
	Astrophys. J., 891, 36-36 (2020)
	Three-dimensional projection effects on chemistry in a Planck galactic cold clump.
o	Figs 3-4, Table 1: <[GMH2020] CN> (Nos C1-C4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMH97]
[GMH97]	(Giannakopoulou+Mitchell+Hasegawa+, 1997)
Write:	<<[GMH97] NN>> <<[GMH97] CNN>>
N:	13+11
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Tables 1, 2: (Nos 1-13), CO intensity peaks in Mon R2 MCld Table 4: (Nos C1-C11), continuum peaks
in source:	NAME Mon R2 GMC
Ref:	=1997ApJ...487..346G
by	GIANNAKOPOULOU J. , MITCHELL G.F., HASEGAWA T.I., MATTHEWS H.E., MAILLARD J.P.
	Astrophys. J., 487, 346-364 (1997)
	The star-forming core of Monoceros R2.
o	Tables 1, 2: <[GMH97] NN> (Nos 1-13). Table 4: <[GMH97] CNN> (Nos C1-C11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMK2001]
[GMK2001]	(Goudfrooij+Mack+Kissler-Patig+, 2001)
Write:	<<[GMK2001] NNN>>
N:	22+19
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	See also [GAM2001b].
in source:	NGC 1316
Ref:	=2001MNRAS.322..643G
by	GOUDFROOIJ P. , MACK J., KISSLER-PATIG M., MEYLAN G., MINNITI D.
	Mon. Not. R. Astron. Soc., 322, 643-657 (2001)
	Kinematics, ages and metallicities of star clusters in NGC 1316: a 3-Gyr-old merger remnant.
o	Globular clusters in NGC 1316. Some objects are stars.
o	Table 2: <[GMK2001] NNN> N=22 among (Nos 103-126), N=17 among (Nos 202-220).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GML2004]
[GML2004]	(Ganesalingam+Moore+Li+, 2004)
Write:	<<[GML2004] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	LOSS observations on KAIT. Host galaxy of SN 2004DZ.
Ref:	=2004IAUC.8395....3G
by	GANESHALINGAM M. , MOORE M., LI W.
	IAU Circ., 8395, 3-None (2004)
	Supernovae 2004dy and 2004dz.
o	<[GML2004] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GML2019]
[GML2019]	(Gonzalez-Lopezlira+Mayya+Loinard+, 2019)
Write:	<<[GML2019] JHHMMSS+DDMMSS>>
N:	11
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	GTC OSIRIS spectroscopy of N=11 sources in NGC 4258. See also GLL.
in source:	NGC 4258
Ref:	=2019ApJ...876...39G
by	GONZALEZ-LOPEZLIRA R.A. , MAYYA Y.D., LOINARD L., ALAMO-MARTINEZ K., HEALD G., GEORGIEV I.Y., ORDENES-BRICENO Y., LANCON A., LARA-LOPEZ M.A., LOMELI-NUNEZ L., BRUZUAL G., PUZIA T.H.
	Astrophys. J., 876, 39-39 (2019)
	Spectroscopy of NGC 4258 globular cluster candidates: membership confirmation and kinematics.
o	Table 2: <[GML2019] JHHMMSS+DDMMSS> N=11, <GLL JHHMMSS+DDMMSS> N=2 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GML92]
[GML92]	(Goldschmidt+Miller+La Franca+, 1992)
Write:	<<[GML92] HHMMSS.s+DDMMSS>>
N:	12
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	N=12 UVX quasars from the Edinburgh Survey
Ref:	=1992MNRAS.256p..65G
by	GOLDSCHMIDT P. , MILLER L., LA FRANCA F., CRISTIANI S.
	Mon. Not. R. Astron. Soc., 256, part no 16, 65-68 (1992)
	The high surface density of bright ultraviolet-excess quasars.
o	Table 1: <[GML92] HHMMSS.s-DDMMSS> N=12
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GMM
GMM	(Glass+Moneti+Moorwood)= ([GMM90])
Write:	<<GMM NN>>
N:	15
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	See also MGM
in source:	NAME Quintuplet Cluster
Ref:	=1990MNRAS.242p..55G
by	GLASS I.S. , MONETI A., MOORWOOD A.F.M.
	Mon. Not. R. Astron. Soc., 242, part no 16, 55-58 (1990)
	Infrared images and photometry of the cluster near G 0.15-0.05.
o	Erratum in MNRAS.244.767, 1990
o	Fig.1, Tables 1, 2: <GMM NN> (Nos 1-15).
Origin	of the Acronym: L (1999MNRAS.304L..10G)
Details on Acronym: [GMM2000]
[GMM2000]	(Guerrero+Miranda+Manchado+, 2000) (Not yet in Simbad)
Write:	<<[GMM2000] A>> <<[GMM2000] A'>>
N:	3+3
Object:	Feature (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Morphological study of NGC 6891: Symmetrical features A-A', B-B', and C'C'.
in source:	NGC 6891
Ref:	=2000MNRAS.313....1G
by	GUERRERO M.A. , MIRANDA L.F., MANCHADO A., VAZQUEZ R.
	Mon. Not. R. Astron. Soc., 313, 1-7 (2000)
	The triple-shell structure and collimated outflows of the planetary nebula NGC 6891.
o	Figs 1, 2, 5: <[GMM2000] A> (Nos A-C), <[GMM2000] A'> (Nos A'-C').
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMM2006]
[GMM2006]	(Gezari+Martin+Milliard+, 2006)
Write:	<<[GMM2006] JHHMMSS.s+DDMMSS>>
N:	1
Object:	UV flare (SIMBAD class: UV = UV-emission Source)
Note:	N=1 luminous UV flare in the Groth field of the GALEX Deep Imaging Survey.
Ref:	=2006ApJ...653L..25G
by	GEZARI S. , MARTIN D.C., MILLIARD B., BASA S., HALPERN J.P., FORSTER K., FRIEDMAN P.G., MORRISSEY P., NEFF S.G., SCHIMINOVICH D., SEIBERT M., SMALL T., WYDER T.K.
	Astrophys. J., 653L, 25-28 (2006)
	Ultraviolet detection of the tidal disruption of a star by a supermassive black hole.
o	In the abstract, elliptical galaxy at z = 0.37 is [HSP2005] J141928.768+525153.34 in SIMBAD.
o	Text: <[GMM2006] JHHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMM2008]
[GMM2008]	(Gutermuth+Myers+Megeath+, 2008)= ([GMM2008a])
Write:	<<[GMM2008] NNN>>
N:	186
Object:	(IR) (SIMBAD class: YSO = Young Stellar Object)
Note:	Spitzer observations of NGC 1333. See also [WMW2010], [WMW2007].
in source:	NGC 1333
Ref:	=2008ApJ...674..336G
by	GUTERMUTH R.A. , MYERS P.C., MEGEATH S.T., ALLEN L.E., PIPHER J.L., MUZEROLLE J., PORRAS A., WINSTON E., FAZIO G.
	Astrophys. J., 674, 336-356 (2008)
	Spitzer observations of NGC 1333: a study of structure and evolution in a nearby embedded cluster.
o	Table 2: <[GMM2008] NNN> (Nos 1-137).
Ref:	=2010AJ....140..266W
by	WINSTON E. , MEGEATH S.T., WOLK S.J., SPITZBART B., GUTERMUTH R., ALLEN L.E., HERNANDEZ J., COVEY K., MUZEROLLE J., HORA J.L., MYERS P.C., FAZIO G.G.
	Astron. J., 140, 266-292 (2010)
	The properties of X-ray luminous young stellar objects in the NGC 1333 and Serpens embedded clusters.
o	In paragraph 4 BD-24607 is a probable misprint for BD-02 4601.
o	Table 1: <[WMW2010] NNN> N=180 among (Nos 1-192). Table 3: <[GMM2008] NNN> (Nos 138-186) added.
=E=	Catalogue in electronic form as J/ApJ/674/336
=E=	Catalogue in electronic form as <J/AJ/140/266/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMM2008a]
[GMM2008a]	(Gutermuth+Myers+Megeath+, 2008)
*****	Avoid the usage of [GMM2008a], prefer [GMM2008]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMM2008b]
[GMM2008b]	(Goncalves+Magrini+Murani+, 2008)
Write:	<<[GMM2008b] IC10 SySt-N>> <<[GMM2008b] A>>
N:	1+5
Object:	* (SIMBAD class: Star)
Note:	Gemini North GMOS observations of IC 10. Detection of a symbiotic star (SySt).
in source:	IC 10
Ref:	=2008MNRAS.391L..84G
by	GONCALVES D.R. , MAGRINI L., MUNARI U., CORRADI R.L.M., COSTA R.D.D.
	Mon. Not. R. Astron. Soc., 391L, 84-87 (2008)
	Discovery in IC10 of the farthest known symbiotic star.
o	Text: <[GMM2008b] IC10 SySt-1> N=1. Table 1, Fig.2: <[GMM2008b] A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMM2009]
[GMM2009]	(Gutermuth+Megeath+Myers+, 2009)= ([GMM2009a])
Write:	<<[GMM2009] AFGLNNN NNN>> <<[GMM2009] BD +DD NNNN NN>> <<[GMM2009] CBNN NN>> <<[GMM2009] Cep A NN>> <<[GMM2009] Cha R NN>> <<[GMM2009] CrA NN>> <<[GMM2009] GGD NN NN>> <<[GMM2009] GGD NN-NN NNN>> <<[GMM2009] ICNNN NNN>> <<[GMM2009] IRAS HHMMm+DDMM NNN>> <<[GMM2009] LNNNN NN>> <<[GMM2009] L988-e NN>> <<[GMM2009] LkHANNN NNN>> <<[GMM2009] Lupus R NN>> <<[GMM2009] Mon RN NNN>> <<[GMM2009] MWCNNN NN>> <<[GMM2009] NGC NNNN NNN>> <<[GMM2009] Oph LNNNN NNN>> <<[GMM2009] SNNN NN>> <<[GMM2009] S140-North NN>> <<[GMM2009] Serpens NN>> <<[GMM2009] Tau LNNNN NN>> <<[GMM2009] VY Mon NN>> <<[GMM2009] XY Per N>>
N:	2750
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC and MIPS observations of N=2548 YSOs in 36 young, nearby clusters.
Ref:	=2009ApJS..184...18G
by	GUTERMUTH R.A. , MEGEATH S.T., MYERS P.C., ALLEN L.E., PIPHER J.L., FAZIO G.G.
	Astrophys. J., Suppl. Ser., 184, 18-83 (2009)
	A Spitzer survey of young stellar clusters within one kiloparsec of the Sun: cluster core extraction and basic structural analysis.
o	(Erratum) erratum vol. 189, p. 352 (2010)
o	Table 4: <[GMM2009] AFGL490 NNN> (Nos 1-161), <[GMM2009] BD+40 4124 NN> (Nos 1-34), <[GMM2009] CB34 NN> (Nos 1-23), <[GMM2009] Cep A NNN> (Nos Cep A 1 to Cep A 96, Cep C 1 to Cep C 114), <[GMM2009] Cha I NN> (Nos 1-38), <[GMM2009] CrA NN> (Nos 1-35), <[GMM2009] GGD NN NN> (Nos GGD 4 1 to GGD 4 31, GGD 17 1 to GGD 17 53), <[GMM2009] GGD 12-15 NNN> (Nos 1-119), <[GMM2009] ICNNNN NNN> (Nos IC348 1 to 160, IC 5146 1 to 149), <[GMM2009] IRAS HHMMm+DDMM NNN> (Nos IRAS 06046-0603 1 to 26, IRAS 20050+2720 1 to 177), <[GMM2009] LNNNN NN> (Nos L1206 1 to 25, L1211 1 to 64), <[GMM2009] L988-e NN> (Nos 1-80), <[GMM2009] LkHA 101 NNN> (Nos 1-103), <[GMM2009] Lupus III NN> (Nos 1-39), <[GMM2009] Mon R2 NNN> (Nos 1-235), <[GMM2009] MWC 297 NN> (Nos 1-23), <[GMM2009]NGC NNNN NNN> (Nos NGC 1333 1 to 133, NGC 7129 1 to 58), <[GMM2009] Oph LNNNN NNN> (Nos Oph L1688 1 to 147, Oph L1689 1 to 5, Oph L1709 1 to 3), <[GMM2009] SNNN NN> (Nos S106 1 to 79, S131 1 to 13, S140 1 to 48, S171 1 to 48), <[GMM2009] S140-North NN> (Nos 1-24), <[GMM2009] Serpens NN> (Nos 1-97), <[GMM2009] Tau LNNNN NN> (Nos Tau L1495 1 to 39, Tau L1551 1 to 13), <[GMM2009] VY Mon NN> (Nos 1-49), <[GMM2009] XY Per N> (Nos 1-7).
Ref:	=2012ApJ...752..127M
by	MASIUNAS L.C. , GUTERMUTH R.A., PIPHER J.L., MEGEATH S.T., MYERS P.C., ALLEN L.E., KIRK H.M., FAZIO G.G.
	Astrophys. J., 752, 127 (2012)
	A structural analysis of star-forming region AFGL 490.
o	Table 1: <[GMM2009] AFGL490 NNN> (Nos 162-363) added.
=E=	Catalogue in electronic form as J/ApJS/184/18
=E=	Catalogue in electronic form as J/ApJ/752/127
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMM2009a]
[GMM2009a]	(Gutermuth+Megeath+Myers+, 2009)
Note:	Spitzer IRAC and MIPS observations of N=2548 YSOs in 36 young, nearby clusters.
*****	Avoid the usage of [GMM2009a], prefer [GMM2009]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMM2009b]
[GMM2009b]	(Guo+McIntosh+Mo+, 2009)
Write:	<<[GMM2009b] NYU-VAGC NNNNNNN>>
N:	2046+1095+1091
Object:	G (SIMBAD class: Galaxy)
Note:	Galaxies selected from the SDSS DR4, using the NYU-VAGC (New York University Value-Added Galaxy Catalog, http://sdss.physics.nyu.edu/vagc/). See also [MGH2008].
Ref:	=2009MNRAS.398.1129G
by	GUO Y. , McINTOSH D.H., MO H.J., KATZ N., VAN DEN BOSCH F.C., WEINBERG M., WEINMANN S.M., PASQUALI A., YANG X.
	Mon. Not. R. Astron. Soc., 398, 1129-1149 (2009)
	Structural properties of central galaxies in groups and clusters.
o	Tables B1-B3: <[GMM2009b] NYU-VAGC NNNNNNN> N=2046 among (Nos 713-1116510).
Ref:	=2017MNRAS.464.3882W
by	WESTON M.E. , McINTOSH D.H., BRODWIN M., MANN J., COOPER A., McCONNELL A., NIELSEN J.L.
	Mon. Not. R. Astron. Soc., 464, 3882-3906 (2017)
	Incidence of WISE-selected obscured AGNs in major mergers and interactions from the SDSS.
o	Table 2: <[GMM2009b] NYU-VAGC NNNNNNN> N=1095 added among (Nos 712-1116117).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMM2012]
[GMM2012]	(Goncalves+Magrini+Martins+, 2012)
Write:	<<[GMM2012] NN>>
N:	15
Object:	Em. Obj. (SIMBAD class: EmObj = Emission Object)
Note:	Gemini North telescope GMOS observations of N=15 emission-line objects in NGC 185.
in source:	NGC 185
Ref:	=2012MNRAS.419..854G
by	GONCALVES D.R. , MAGRINI L., MARTINS L.P., TEODORESCU A.M., QUIREZA C.
	Mon. Not. R. Astron. Soc., 419, 854-865 (2012)
	Deep spectroscopy of the emission-line populations in NGC 185.
o	Table 1: <[GMM2012] NN> (Nos 1-15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMM90]
[GMM90]	(Glass+Moneti+Moorwood, 1990)
*****	Avoid the usage of [GMM90], prefer GMM
Origin	of the Acronym: S = Created by Simbad, the CDS Database
History	of this Acronym: replaced by GMM
Details on Acronym: [GMN2017]
[GMN2017]	(Ginolfi+Maiolino+Nagao+, 2017)
Write:	<<[GMN2017] N>>
N:	9
Object:	G (SIMBAD class: Galaxy)
Note:	ALMA Cycle 1 band 3 CO(4-3) line observations of N=5 CO emission systems around the massive star-forming galaxy Candels-5001 at z=3.47 within the GOODS-S field.
Ref:	=2017MNRAS.468.3468G
by	GINOLFI M. , MAIOLINO R., NAGAO T., CARNIANI S., BELFIORE F., CRESCI G., HATSUKADE B., MANNUCCI F., MARCONI A., PALLOTTINI A., SCHNEIDER R., SANTINI P.
	Mon. Not. R. Astron. Soc., 468, 3468-3483 (2017)
	Molecular gas on large circumgalactic scales at z = 3.47.
o	Table D1: <[GMN2017] N> (Nos 0-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GMP
GMP	(Godwin+Metcalfe+Peach)= (GMP83)
Write:	<<GMP NNNN>>
N:	6724
Object:	G (SIMBAD class: Galaxy)
Note:	On microfiches MN 202/1 and 2
in source:	Coma Cluster = ACO 1656
Ref:	=1983MNRAS.202..113G
by	GODWIN J.G. , METCALFE N., PEACH J.V.
	Mon. Not. R. Astron. Soc., 202, 113-124 (1983)
	The Coma Cluster - I. A Catalogue of magnitudes, colours, ellipticies and position angles for 6724 galaxies in the field of the Coma Cluster.
o	Appendix: <GMP NNNN> (Nos 1-6724)
=E=	Catalogue in electronic form as VII/42
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GMP2000]
[GMP2000]	(Guirado+Marcaide+Perez-Torres+, 2000)= ([GMP2000a]) (Not yet in Simbad)
Write:	<<[GMP2000] QSO 1928+738 QN>> <<[GMP2000] QSO 2007+777 QN>>
N:	1+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Fig.1: (No. Q1) in QSO 1928+738 is the brightest knot (a jet component). (Nos Q1-Q2)in QSO 2007+777 are the brightest components. See also [JSE87], [HSK92], [GMR98b].
in source:	QSO B1928+738
in source:	QSO B2007+777
Ref:	=2000A&A...353L..37G
by	GUIRADO J.C. , MARCAIDE J.M., PEREZ-TORRES M.A., ROS E.
	Astron. Astrophys., 353, 37-40 (2000)
	VLBI difference astrometry at 43GHz.
o	Fig.1: <[GMP2000] QSO 1928+738 QN> (No. Q1), <[GMP2000] QSO 2007+777 QN> (Nos Q1-Q2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMP2000a]
[GMP2000a]	(Guirado+Marcaide+Perez-Torres+, 2000) (Not yet in Simbad)
*****	Avoid the usage of [GMP2000a], prefer [GMP2000]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMP2000b]
[GMP2000b]	(Garcia+Murray+Primini+, 2000)
Write:	<<[GMP2000b] JHHMMSS.s+DDMMSS.s>>
N:	1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations. X-ray transient, apparently within M 32.
in source:	M 32
Ref:	=2000IAUC.7498S...1G
by	GARCIA M.R. , MURRAY S.S., PRIMINI F.A., McCLINTOCK J.E., CALLANAN P.J.
	IAU Circ., 7498, 1-None (2000)
	X-ray transient in M 32.
o	<[GMP2000b] JHHMMSS.s+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMP2005]
[GMP2005]	(Giannini+Massi+Podio+, 2005)
Write:	<<[GMP2005] mmA>>
N:	2
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	SEST SIMBA 1.2mm observations. N=2 peaks of 1.2mm continuum emission in VMR.
in source:	NAME VMR
Ref:	=2005A&A...433..941G
by	GIANNINI T. , MASSI F., PODIO L., LORENZETTI D., NISINI B., CARATTI O GARATTI A., LISEAU R., LO CURTO G., VITALI F.
	Astron. Astrophys., 433, 941-954 (2005)
	Star formation in the Vela Molecular Clouds: A new protostar powering a bipolar jet.
o	Figs: <[LGV2002] IRS NN AN> N=6 added, <[LGV2002] IRS 40 N> (Nos 1-6). Table 7: <[GMP2005] mmA> (Nos mmA, mmB).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMP2008]
[GMP2008]	(Gusev+Myakutin+Piskunov+, 2008) (Not yet in Simbad)
Write:	<<[GMP2008] NGC NNNN NN>> <<[GMP2008] NGC 4656-57 NN>>
N:	24+79+26+36+9
Object:	Star Forming Complex (SIMBAD class: Region = Region defined in the Sky)
Note:	Search for Star-Formation Complexes in five galaxies.
in source:	NGC 1068
in source:	NGC 4449
in source:	NGC 4490
in source:	NGC 4631
in source:	NGC 4656
in source:	NGC 4657
Ref:	=2008ARep...52..714G
by	GUSEV A.S. , MYAKUTIN V.I., PISKUNOV A.E., SAKHIBOV F.K., KHRAMTSOVA M.S.
	ARep, 52, 714-728 (2008)
	Age and interstellar absorption in young star-formation regions in the galaxies NGC 1068, NGC 4449, NGC 4490, NGC 4631, and NGC 4656/57 derived from multicolor photometry.
o	2008AZh....85..794G
o	Table 1, Figs 3: <[GMP2008] NGC 1068 NN> (Nos 1-24), <[GMP2008] NGC 4449 NN> (Nos 1-79), <[GMP2008] NGC 4490 NN> N=26 among (Nos 2-32), <[GMP2008] NGC 4631 NN> N=36 among (Nos 1-53), <[GMP2008] NGC 4656-57 NN> N=9 among (Nos 4-26).
=E=	Catalogue in electronic form as J/AZh/85/794
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMP2010]
[GMP2010]	(Guarcello+Micela+Peres+, 2010)
Write:	<<[GMP2010] NNNN>>
N:	2227
Object:	* (SIMBAD class: Star)
Note:	N=2227 stars in NGC 6611. Use of Chandra ACIS, UKIDSS, EIS and Spitzer IRAC data. See also Cl* NGC 6611 GPM, Cl* NGC 6611 GMD, [GDM2010].
in source:	Eagle Nebula = NGC 6611 = M 16
Ref:	=2010A&A...521A..61G
by	GUARCELLO M.G. , MICELA G., PERES G., PRISINZANO L., SCIORTINO S.
	Astron. Astrophys., 521A, 61-61 (2010)
	Chronology of star formation and disk evolution in the Eagle Nebula.
o	m16memb: <[GMP2010] NNNN> (Nos 1-2227).
=E=	Catalogue in electronic form as J/A+A/521/A61
Details on Acronym: [GMP2019]
[GMP2019]	(Gilli+Mignoli+Peca+, 2019)
Write:	<<[GMP2019] mN>> <<[GMP2019] lN>> <<[GMP2019] A>> <<[GMP2019] J1030 overdensity>>
N:	6+2+4+1
Object:	G + (X) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT MUSE observations of N=6 galaxies and LBT LUCI observations of N=2 galaxies in N=1 galaxy overdensity, in the field of QSO J1030+0524. Chandra ACIS observations of N=4 diffuse X-ray sources, also in the field of QSO J1030+0524. See also [DGP2020].
Ref:	=2019A&A...632A..26G
by	GILLI R. , MIGNOLI M., PECA A., NANNI R., PRANDONI I., LIUZZO E., D'AMATO Q., BRUSA M., CALURA F., CAMINHA G.B., CHIABERGE M., COMASTRI A., CUCCIATI O., CUSANO F., GRANDI P., DECARLI R., LANZUISI G., MANNUCCI F., PINNA E., TOZZI P., VANZELLA E., VIGNALI C., VITO F., BALMAVERDE B., CITRO A., CAPPELLUTI N., ZAMORANI G., NORMAN C.
	Astron. Astrophys., 632A, 26-26 (2019)
	Discovery of a galaxy overdensity around a powerful, heavily obscured FRII radio galaxy at z = 1.7: star formation promoted by large-scale AGN feedback?
o	XID 189 not identified.
o	<[GMP2019] J1030 overdensity> N=1. Figs 1+8, Table 1: <[GMP2019] mN> (Nos m1-m6), <[GMP2019] lN> (Nos l1-l2). Fig. 9, Table 2: <[GMP2019] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GMP83
GMP83	(Godwin+Metcalfe+Peach, 1983)
*****	Avoid the usage of GMP83, prefer GMP
Origin	of the Acronym: L (2001AJ....121.2331C)
Details on Acronym: [GMP90]
[GMP90]	(Garcia-Lario+Manchado+Pottasch+, 1990) (Not yet in Simbad)
Write:	<<[GMP90] NN>>
N:	42
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	See also paper III: GLMP
Ref:	=1990A&AS...82..497G
by	GARCIA-LARIO P. , MANCHADO A., POTTASCH S.R., SUSO J., OLLING R.
	Astron. Astrophys., Suppl. Ser., 82, 497-512 (1990)
	Near infrared survey of IRAS sources with colours like planetary nebulae. II.
o	Table 1: <[GMP90] NN> (Nos 1-42).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GMP94]
[GMP94]	(Garmany+Massey+Parker, 1994)
Write:	<<[GMP94] NNN>>
N:	839
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1994AJ....108.1256G
by	GARMANY C.D. , MASSEY P., PARKER J.W.
	Astron. J., 108, 1256-1265 (1994)
	The OB association LH 58 in the Large Magellanic Cloud.
o	Table 3 is presented in its complete form in the ApJ/AJ CD-ROM Series, Vol.3, 1994
o	Table 3: <[GMP94] NNN> N=839
=E=	Catalogue in electronic form as J/AJ/108/1256
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GMR
GMR	(Garay+Maran+Reid)= (CFWM) = (FTCCK) = (VLA)
Write:	<<GMR NN>> <<GMR A>>
N:	26+18
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio-sources in Orion nebula (format 'NN' in Trapezium)
in source:	NAME Orion Nebula
Ref:	=1987ApJ...314..535G
by	GARAY G. , MORAN J.M., REID M.J.
	Astrophys. J., 314, 535-550 (1987)
	Compact continuum radio sources in the Orion nebula.
o	Table 2: <GMR NN> (Nos 1-14). Table 3: <GMR A> (Nos A-G).
Ref:	=1987ApJ...321..516C
by	CHURCHWELL E. , FELLI M., WOOD D.O.S., MASSI M.
	Astrophys. J., 321, 516-529 (1987)
	Solar system-sized condensations in the Orion nebula.
o	Table 1: <GMR NN> (Nos 15-18) added, <GMR A> (Nos H-K) added.
Ref:	=1993A&AS..101..127F
by	FELLI M. , TAYLOR G.B., CATARZI M., CHURCHWELL E., KURTZ S.
	Astron. Astrophys., Suppl. Ser., 101, 127-151 (1993)
	The Orion radio zoo revisited: source variability.
o	Table 1: <GMR NN> (Nos 19-26) added, <GMR A> (Nos L-R) added.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GMR2000]
[GMR2000]	(Ghosh+Mookerjea+Rengarajan+, 2000)
Write:	<<[GMR2000] SNN>>
Object:	(FIR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Balloon-borne TIFR observations, IRAS and ISO LWS data. Far IR sources in the field of IRAS 09002-4732.
Ref:	=2000A&A...363..744G
by	GHOSH S.K. , MOOKERJEA B., RENGARAJAN T.N., TANDON S.N., VERMA R.P.
	Astron. Astrophys., 363, 744-754 (2000)
	Far infrared observations of the southern Galactic star forming complex around IRAS 09002-4732.
o	Table 2: <[GMR2000] SNN> (Nos S1-S15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMR2009]
[GMR2009]	(Gregorio-Hetem+Montmerle+Rodrigues+, 2009)
Write:	<<[GMR2009] CMaX NN>> <<[GMR2009] CMaX NNW>> <<[GMR2009] CMaX NNWN>> <<[GMR2009] CMaX NN-N>>
N:	98+4+10+2
Object:	Unknown (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Gemini South telescope observations of ROSAT fields around the CMA R1 star-forming region. Use of archival ROSAT images.
in source:	NAME ASS CMA R 1-
Ref:	=2009A&A...506..711G
by	GREGORIO-HETEM J. , MONTMERLE T., RODRIGUES C.V., MARCIOTTO E., PREIBISCH T., ZINNECKER H.
	Astron. Astrophys., 506, 711-727 (2009)
	Star formation history of Canis Major R1. I. Wide-field X-ray study of the young stellar population.
o	Tables A.1, A.2: <[GMR2009] CMaX NN> (Nos 1-98). Table 1: <[GMR2009] CMaX NNW> (Nos 17N, 17S, 55N ,55S). Table 2: <[GMR2009] CMaX NN-N>, <[GMR2009] CmaX NNWN> N=17.
=E=	Catalogue in electronic form as J/A+A/506/711
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMR2016]
[GMR2016]	(Gomez-Gonzalez+Mayya+Rosa-Gonzalez, 2016)
Write:	<<[GMR2016] WRNN>>
N:	21
Object:	WR (SIMBAD class: WolfRayet* = Wolf-Rayet)
Stat.	in SIMBAD: Ref. 2016MNRAS.460.1555G is completely incorporated.
Note:	GTC OSIRIS spectroscopic observations of N=21 stars in M81. Use of archival HST images.
in source:	NGC 3031 = M 81
Ref:	=2016MNRAS.460.1555G
by	GOMEZ-GONZALEZ V.M.A. , MAYYA Y.D., ROSA-GONZALEZ D.
	Mon. Not. R. Astron. Soc., 460, 1555-1566 (2016)
	Wolf-Rayet stars in M81: detection and characterization using GTC/OSIRIS spectra and HST/ACS images.
o	Table 2: the 'kaufNNN' (=[KBK87] NNN) complex are not in SIMBAD.
o	Table 2: <[GMR2016] WRNN> (Nos 1-14).
Ref:	=2020MNRAS.493.3879G
by	GOMEZ-GONZALEZ V.M.A. , MAYYA Y.D., ROSA-GONZALEZ D., RODRIGUEZ-MERINO L.H., TOALA J.A., ALVAREZ C.
	Mon. Not. R. Astron. Soc., 493, 3879-3892 (2020)
	Wolf-Rayet stars in M 81 using GTC/OSIRIS: seven new detections, analysis, and classification of the full sample.
o	Figs 2-3, Table 2: <[GMR2016] WRNN> (Nos 15-21) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMR67]
[GMR67]	(Gardner+McGee+Robinson, 1967)
Write:	<<[GMR67] A>>
N:	2
Object:	Em. source (SIMBAD class: EmObj = Emission Object)
Stat:	is completely incorporated in Simbad
Note:	N=2 OH-line emission sources in NGC 6334.
in source:	NGC 6334
Ref:	=1967AuJPh..20..309G
by	GARDNER F.F. , McGEE R.X., ROBINSON B.J.
	Australian J. Phys., 20, 309-324 (1967)
	18cm OH-line radiation from NGC 6334.
o	Plate 2: <[GMR67] A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMR92]
[GMR92]	(Gwinn+Moran+Reid, 1992)
Write:	<<[GMR92] NNN>>
N:	105
Object:	H2O Maser (SIMBAD class: Maser)
in source:	W 49:W 49N = W 49N
Ref:	=1992ApJ...393..149G
by	GWINN C.R. , MORAN J.M., REID M.J.
	Astrophys. J., 393, 149-164 (1992)
	Distance and kinematics of the W 49N H2O maser outflow.
o	<[GMR92] NNN> N=105
=E=	Catalogue in electronic form as J/ApJ/393/149
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMR98]
[GMR98]	(Garay+Moran+Rodriguez+, 1998)= ([GMR98a])
Write:	<<[GMR98] HII A>> <<[GMR98] HII AA>> <<[GMR98] Clump A>> <<[GMR98] Clump WW>>
N:	5+3
Object:	HII + Clump (SIMBAD class: ISM = Interstellar Medium Object)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=5 HII regions in the region Gal 19.6-0.2 (Nos A, B, CD, E, F). Table 4: N=3 clumps in the region Gal 19.6-0.2 (Nos M, N, SW) where 'M' stands for 'Middle'.
Ref:	=1998ApJ...492..635G
by	GARAY G. , MORAN J.M., RODRIGUEZ L.F., REID M.J.
	Astrophys. J., 492, 635-649 (1998)
	The G19.6-0.2 region of star formation: molecular and ionized environs.
o	Table 2: <[GMR98] HII A>, <[GMR98] HII AA>, (Nos A, B, CD, E, F). Table 4: <[GMR98] Clump WW> (Nos M, N, SW)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMR98a]
[GMR98a]	(Garay+Moran+Rodriguez+, 1998)
*****	Avoid the usage of [GMR98a], prefer [GMR98a]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMR98b]
[GMR98b]	(Guirado+Marcaide+Ros+, 1998) (Not yet in Simbad)
Write:	<<[GMR98b] 1928+738 XN>> <<[GMR98b] 2007+777 SN>>
N:	5+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	See also [JSE87], [HSK92], [GMP2000].
in source:	QSO B1928+738
in source:	QSO B2007+777
Ref:	=1998A&A...336..385G
by	GUIRADO J.C. , MARCAIDE J.M., ROS E., RATNER M.I., SHAPIRO I.I., QUIRRENBACH A., WITZEL A.
	Astron. Astrophys., 336, 385-392 (1998)
	Submilliarcsecond shift of the brightness peak of the radio sources 1928+738 and 2007+777.
o	Fig.1: <[GMR98b] 1928+738 XN> (Nos X1-X5), <[GMR98b] 2007+777 SN> (No. S1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GMRT
GMRT	(Giant Metrewave Radio Telescope)
*****	Avoid the usage of GMRT, prefer [ACG2016]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GMRT
GMRT	(Giant Metrewave Radio Telescope)
*****	Avoid the usage of GMRT, prefer [GS2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GMRT
GMRT	(Giant Metrewave Radio Telescope)
*****	Avoid the usage of GMRT, prefer [GVB2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GMRT
GMRT	(Giant Metrewave Radio Telescope)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GMRT
GMRT	(Giant Metrewave Radio Telescope)
*****	Avoid the usage of GMRT, prefer [PMI2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GMRT
GMRT	(Giant Metrewave Radio Telescope)
*****	Avoid the usage of GMRT, prefer [PMI2009]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GMRT
GMRT	(Giant Metrewave Radio Telescope)
*****	Avoid the usage of GMRT, prefer [SSI2009]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GMRT
GMRT	(Giant Metrewave Radio Telescope)
*****	Avoid the usage of GMRT, prefer [VRB2017]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GMRTEN1
GMRTEN1	(Giant Metrewave Radio Telescope, ELAIS-N1 survey)
Write:	<<GMRTEN1 JHHMMSS.s+DDMMSS>>
N:	2500
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	GMRT 610MHz observations of the ELAIS N1 field.
in source:	ELAIS N1
Ref:	=2008MNRAS.383...75G
by	GARN T. , GREEN D.A., RILEY J.M., ALEXANDER P.
	Mon. Not. R. Astron. Soc., 383, 75-85 (2008)
	A 610-MHz survey of the ELAIS-N1 field with the Giant Metrewave Radio Telescope - observations, data analysis and source catalogue.
o	Catalog: <GMRTEN1 JHHMMSS.s+DDMMSS> N=2500.
=E=	Catalogue in electronic form as J/MNRAS/383/75
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: GMRTLH
GMRTLH	(Giant Metrewave Radio Telescope, Lockman Hole)
Write:	<<GMRTLH JHHMMSS.s+DDMMSS>>
N:	2845+4934
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Oservations of the Lockman Hole with the Giant Metrewave Radio Telescope (GMRT). Twelve pointings were observed, covering a total area of about five square degrees with a resolution of 6x5 arcsec, position angle +45deg. The majority of the pointings have an rms noise of 60 microJy per beam before correction for the attenuation of the GMRT primary beam. Techniques used for data reduction and production of a mosaicked image of the region are described, and the final mosaic is presented, along with a catalogue of 2845 sources detected above 6 sigma. Radio source counts are calculated at 610 MHz and combined with existing 1.4-GHz source counts, in order to show that pure luminosity evolution of the local radio luminosity functions for active galactic nuclei and starburst galaxies is sufficient to account for the two source counts simultaneously.
in source:	NAME Lockman Hole
Ref:	=2008MNRAS.387.1037G
by	GARN T. , GREEN D.A., RILEY J.M., ALEXANDER P.
	Mon. Not. R. Astron. Soc., 387, 1037-1044 (2008)
	A 610-MHz survey of the Lockman Hole with the Giant Metrewave Radio Telescope - I. Observations, data reduction and source catalogue for the central 5 °^{2}.
o	Table 1: <GMRTLH JHHMMSS.s+DDMMSS> N=2845.
Ref:	=2010BASI...38..103G
by	GARN T.S. , GREEN D.A., RILEY J.M., ALEXANDER P.
	BASI, 38, 103-112 (2010)
	Further GMRT observations of the Lockman Hole at 610 MHz.
o	Table 1: <GMRTLH JHHMMSS.s+DDMMSS> N=4934. Astrophysics Group, University of Cambridge
=E=	Catalogue in electronic form as J/MNRAS/387/1037
=E=	Catalogue in electronic form as <J/other/BASI/38.103/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [GMS2007]
[GMS2007]	(Goddi+Moscadelli+Sanna+, 2007) (Not yet in Simbad)
Write:	<<[GMS2007] Sh 2-255 IR NN>> <<[GMS2007] AFGL 5142 NN>>
N:	57+27
Object:	H2O + CH3OH Maser (SIMBAD class: Maser)
Note:	VLBI observations to search for H2O and CH3OH masers toward Sh 2-255 IR and AFGL 5142.
in source:	SH 2-255
in source:	RAFGL 5142
Ref:	=2007A&A...461.1027G
by	GODDI C. , MOSCADELLI L., SANNA A., CESARONI R., MINIER V.
	Astron. Astrophys., 461, 1027-1035 (2007)
	Associations of H_{2}O and CH_{3}OH masers at milli-arcsec angular resolution in two high-mass YSOs.
o	Paragraph 1. G313.77-0.86 is IRAS 14212-6131 in Simbad. Paragraph 2.2. phase-reference source J0518+3306 not identified.
o	Table 1: <[GMS2007] Sh 2-255 IR NN> (Nos 1-57). Table 2: <[GMS2007] AFGL 5142 NN> (Nos 1-27).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMS93]
[GMS93]	(Gaidos+Magnier+Schechter, 1993)
Write:	<<[GMS93] NN>>
N:	25
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Ref:	=1993PASP..105.1294G
by	GAIDOS E.J. , MAGNIER E.A., SCHECHTER P.L.
	Publ. Astron. Soc. Pac., 105, 1294-1307 (1993)
	A catalog of QSO candidates from a BVRI CCD survey of the North Ecliptic Pole.
o	<[GMS93] NN> (Nos 1-25).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMS94]
[GMS94]	(Graham+Matthews+Soifer+, 1994)= (G94) = ([GMS94a])
Write:	<<[GMS94] NN>>
N:	18
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Photometry of 4C 41.17. Plate L4
Ref:	=1994ApJ...420L...5G
by	GRAHAM J.R. , MATTHEWS K., SOIFER B.T., NELSON J.E., HARRISON W., JERNIGAN J.G., LIN S., NEUGEBAUER G., SMITH G., ZIOMKOWSKI C.
	Astrophys. J., 420, 5-8 (1994)
	Infrared observations of the z = 3.8 radio galaxy 4C 41.17 with the W.M. Keck telescope.
o	Table 1: <[GMS94] NN> (Nos 1-18)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMS94a]
[GMS94a]	(Graham+Matthews+Soifer+, 1994)
*****	Avoid the usage of [GMS94a], prefer [GMS94]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMS94b]
[GMS94b]	(Giavalisco+Macchetto+Sparks, 1994)
Write:	<<[GMS94b] GN>>
N:	5
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=5 galaxies towards QSO 0000-2619, (Nos G1-G5). [GMS94b] G1 found has 'G' galaxy in 1991ApJ...382...26T. [GMS94b] G1 , G2 = [MLG93] G1 , G2. Map in Fig.1.
Ref:	=1994A&A...288..103G
by	GIAVALISCO M. , MACCHETTO F.D., SPARKS W.B.
	Astron. Astrophys., 288, 103-121 (1994)
	Narrow-band imaging of fields around optically-thick absorption systems: the line-of-sight towards Q 0000-2619.
o	fig. 4 and text p.107: galaxy A = [SH92] QSO 0000-263 A, T.3: [MLG93] ON
o	Table 2: <[GMS94b] GN> (Nos G1-G5)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMS97]
[GMS97]	(Gosset+Moreau+Surdej+, 1997)
Write:	<<[GMS97] NGC 450 NNN>>
N:	140
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Note:	Table 6: N=140 QSO candidates, among which 59 are QSO, 26 stars, 2 probable stars, 2 G or HII, 1 probable G.
Ref:	=1997A&AS..123..529G
by	GOSSET E. , MOREAU O., SURDEJ J., SWINGS J.P., ARP H.C.
	Astron. Astrophys., Suppl. Ser., 123, 529-568 (1997)
	Surveys of ultraviolet-excess quasar candidates in large fields. The area around NGC 450.
o	Table 6: <[GMS97] NGC 450 NNN> N=140 among (Nos 1-244)
=E=	Catalogue in electronic form as J/A+AS/123/529
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMS99]
[GMS99]	(Gal-Yam+Maoz+Strolger+, 1999)
Write:	<<[GMS99] JHHMMSS.ss+DDMMSS.s>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Wise Observatory observations. Host galaxies of SN 1999AX, SN 1999AY, SN 1999AW.
Ref:	=1999IAUC.7130Q...1G
by	GAL-YAM A. , MAOZ D., STROLGER L.G., SMITH R.C., GOOBAR A., DAHLEN T., HOOK I., NUGENT P.E., PHILLIPS M., LIDMAN C., ALDERING G., DEUSTUA S.
	IAU Circ., 7130, 1-None (1999)
	Supernovae 1999au, 1999av, 1999aw, 1999ax, 1999ay.
o	<[GMS99] JHHMMSS.ss+DDMMSS.s> N=3
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GMT
GMT	(Garilli+Maccagni+Tarenghi)
*****	Avoid the usage of GMT, prefer [GMT93b]
Origin	of the Acronym: L (2001MNRAS.327..265H)
Details on Acronym: [GMT93]
[GMT93]	(Greggio+Marconi+Tosi+, 1993)= ([GMT93a])
Write:	<<[GMT93] DDO 210 ANNN>> <<[GMT93] NGC 3109 ANNNN>>
N:	583+1692
Object:	* (SIMBAD class: Star)
Note:	Table 2: 'DDO 210 ANNN' A for * in regions A or B in DDO 210, region A: N=435, region B: N=148. Table 3: 'NGC 3109 ANNNN' for * in regions A, B, C in NGC 3109, region A: N=1015, region B: N=647, region C: N=930.
in source:	NAME Aquarius Dwarf Galaxy = DDO 210
in source:	NGC 3109
Ref:	=1993AJ....105..894G
by	GREGGIO L. , MARCONI G., TOSI M., FOCARDI P.
	Astron. J., 105, 894-932 (1993)
	Star formation in dwarf irregular galaxies: DDO 210 and NGC 3109.
o	Table 2: <[GMT93] DDO 210 ANNN> N=583. Table 3: <[GMT93] NGC 3109 ANNNN> N=1692
=E=	Catalogue in electronic form as J/AJ/105/894
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMT93a]
[GMT93a]	(Greggio+Marconi+Tosi+, 1993)
*****	Avoid the usage of [GMT93a], prefer [GMT93]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMT93b]
[GMT93b]	(Garilli+Maccagni+Tarenghi, 1993)= (GMT)
Write:	<<[GMT93b] ACO NNNN A>> <<[GMT93b] ACO S NNN A>> <<[GMT93b] Klem 38 A>>
N:	80
Object:	G in ClG (SIMBAD class: Galaxy)
Note:	Format 'ACO S 112 A', N=4 galaxies, (Nos A-D). Format 'ACO 3389 A', N=7 galaxies, (Nos A-G). Format 'ACO S 617 A', N=11 galaxies, (Nos A-K). Format 'ACO S 639 A', N=5 galaxies, (Nos A-E). Format 'ACO 3656 A', N=14 galaxies, (Nos A-N). Format 'ACO 3744 A', N=11 galaxies, (Nos A-K). Format 'ACO S 963 A', N=14 galaxies, (Nos A-N). Format 'Klem 38 A', N=14 galaxies, (Nos A-N).
in source:	ACO S 112
in source:	ACO 3389
in source:	ACO S 617
in source:	ACO S 639
in source:	ACO 3656
in source:	ACO 3744
in source:	ACO S 963
in source:	Klem 38
Ref:	=1993A&AS..100...33G
by	GARILLI B. , MACCAGNI D., TARENGHI M.
	Astron. Astrophys., Suppl. Ser., 100, 33-46 (1993)
	Galaxy velocities in eight southern clusters.
o	Table 2: <[GMT93b] ACO NNNN A> or <[GMT93b] ACO S NNNN A> or <[GMT93b] Klem 38 A> N=80
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMV2014]
[GMV2014]	(Giacintucci+Markevitch+Venturi+, 2014)
Write:	<<[GMV2014] MACS JHHMM.m+DDMM SN>> <<[GMV2014] A NNNN SN>> <<[GMV2014] ZwCl NNNN SN>> <<[GMV2014] ZwCl HHMM.m+DDMM SN>> <<[GMV2014] RX JHHMM.m+DDMM SN>> <<[GMV2014] VLA-JHHMM+DDMM AA>> <<[GMV2014] VLA-JHHMM+DDMM A>>
N:	18+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 1.4GHz, 4.9GHz and 8.5GHz continuum observations of N=18 radio sources in 9 galaxy clusters. Use of archival VLA and GMRT data.
Ref:	=2014ApJ...781....9G
by	GIACINTUCCI S. , MARKEVITCH M., VENTURI T., CLARKE T.E., CASSANO R., MAZZOTTA P.
	Astrophys. J., 781, 9 (2014)
	New detections of radio minihalos in cool cores of galaxy clusters.
o	Table 4: [GMV2014] MACS J1931.8-2634 S1 and [GMV2014] MACS J1931.8-2634 S2 are not in SIMBAD (no coordinates).
o	Table 2: <[GMV2014] MACS JHHMM.m+DDMM SN> N=5, <[GMV2014] A NNNN SN> N=8, <[GMV2014] ZwCl 3146 SN> N=2, <[GMV2014] ZwCl 1742.1+3306 SN> N=2, <[GMV2014] RX J1532.9+3021 SN> N=1. Table 6: <[GMV2014] VLA-J1532+3018 AA> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMV2015]
[GMV2015]	(Geach+More+Verma+, 2015)
Write:	<<[GMV2015] GN>> <<[GMV2015] A>> <<[GMV2015] ASW0009io9>>
N:	5
Object:	Grav. lens + Grav. lensed image of a G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	e-MERLIN and VLA 1.4 and 5GHz observation of a gravitationally lensed hyperluminous infrared galaxy. Use of VISTA NIR data.
Ref:	=2015MNRAS.452..502G
by	GEACH J.E. , MORE A., VERMA A., MARSHALL P.J., JACKSON N., BELLES P.-E., BESWICK R., BAETEN E., CHAVEZ M., CORNEN C., COX B.E., ERBEN T., ERICKSON N.J., GARRINGTON S., HARRISON P.A., HARRINGTON K., HUGHES D.H., IVISON R.J., JORDAN C., LIN Y.-T., LEAUTHAUD A., LINTOTT C., LYNN S., KAPADIA A., KNEIB J.-P., MacMILLAN C., MAKLER M., MILLER G., MONTANA A., MUJICA R., MUXLOW T., NARAYANAN G., O BRIAIN D., O'BRIEN T., OGURI M., PAGET E., PARRISH M., ROSS N.P., ROZO E., RUSU C.E., RYKOFF E.S., SANCHEZ-ARGUELLES D., SIMPSON R., SNYDER C., SCHLOERB F.P., TECZA M., WANG W.-H., VAN WAERBEKE L., WILCOX J., VIERO M., WILSON G.W., YUN M.S., ZEBALLOS M.
	Mon. Not. R. Astron. Soc., 452, 502-510 (2015)
	The Red Radio Ring: a gravitationally lensed hyperluminous infrared radio galaxy at z = 2.553 discovered through the citizen science project Space Warps.
o	Table 1: <[GMV2015] GN> (Nos G1-G2). Fig. 2: <[GMV2015] A> (Nos A-B). Text: <[GMV2015] ASW0009io9>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMV91]
[GMV91]	(Garilli+Maccagni+Vettolani, 1991)
Write:	<<[GMV91] NNN>>
N:	181
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	ACO 3639
Ref:	=1991AJ....101..795G
by	GARILLI B. , MACCAGNI D., VETTOLANI G.
	Astron. J., 101, 795-812 (1991)
	Spectroscopy and multicolour photometry of the medium redshift southern cluster of galaxies A 3639.
o	(Erratum) Erratum: 1993 AJ 105 p. 364
o	Table 1: <[GMV91] NNN> N=181
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMW2004]
[GMW2004]	(Garnavich+Macdonald+Wu+, 2004)
Write:	<<[GMW2004] N>>
N:	3
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VATT observations. N=3 comparison stars in the field of V2275 Cyg nova. Finding chart.
Ref:	=2004IBVS.5519....1G
by	GARNAVICH P.M. , MacDONALD A.J., WU B., EASTERDAY S.M., LIBAL A.J., PALUMBO A., QUINN M.A.
	IAU Inform. Bull. Var. Stars, 5519, 1-None (2004)
	Rapid variations in V2275 Cyg (Nova Cyg 2001#2).
o	Table 1: <[GMW2004] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMW2005]
[GMW2005]	(Gelbord+Marshall+Worall+, 2005) (Not yet in Simbad)
Write:	<<[GMW2005] AN>>
N:	3+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ATCA observations of PKS B1421-490: 3 main emitting regions A to C with A resolved in a pointsource A1 and a jetlike extension A2.
in source:	PKS 1421-490
Ref:	=2005ApJ...632L..75G
by	GELBORD J.M. , MARSHALL H.L., WORRALL D.M., BIRKINSHAW M., LOVELL J.E.J., OJHA R., GODFREY L., SCHWARTZ D.A., PERLMAN E.S., GEORGANOPOULOS M., MURPHY D.W., JAUNCEY D.L.
	Astrophys. J., 632, 75-78 (2005)
	The knotty question of the jet of PKS B1421-490.
o	Fig.1: <[GMW2005] AN> (Nos A-C, A1-A2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GMW2007]
[GMW2007]	(Greissl+Meyer+Wilking+, 2007)
Write:	<<[GMW2007] SN-NN>> <<[GMW2007] SNA-N>>
N:	32
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	HST NICMOS photometry of NGC 1333.
in source:	NGC 1333
Ref:	=2007AJ....133.1321G
by	GREISSL J. , MEYER M.R., WILKING B.A., FANETTI T., SCHNEIDER G., GREENE T.P., YOUNG E.
	Astron. J., 133, 1321-1330 (2007)
	Hubble Space Telescope NICMOS observations of NGC 1333: the ratio of stars to substellar objects.
o	Tables 1 and 3, some coordinates are incorrect. Par. 4.3. : 2MASS 1207-3923 = 2MASS J12073346-3932539.
o	Table 2: <[GMW2007] SN-NN>, <[GMW2007] SNA-N>, N=32.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GN
GN	(GOODS North) (Not yet in Simbad)
*****	Avoid the usage of GN, prefer [LLH2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GN
GN	(G. Nicolson) (Not yet in Simbad)
*****	Avoid the usage of GN, prefer [N65]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: GN
GN	(Gal. Nebula)
Write:	<<GN HH.MM.m>> <<GN HH.MM.m.NN>>
Object:	Neb. Obj. (SIMBAD class: ISM = Interstellar Medium Object)
Note:	Atlas of Galactic Nebulae, Vol. I, II, III, Treugesel-Verlag K.G., D-4000 Dusseldorf 1, 1985, 1987, 1990. Formats 'HH.MM.m' and 'HH.MM.m.NN' where NN is a running number when several objects have similar RA. Some objects are PN, named NeVe, in 1992, Acker+ catalog
Auth.:	NECKEL Th.+
Origin	of the Acronym: L = Found in the literature
Details on Acronym: GN
GN	(GOODS North)
*****	Avoid the usage of GN, prefer [GPS2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GN
GN	(GOODS North)
*****	Avoid the usage of GN, prefer [PBS2005]
Origin	of the Acronym: L (2007ApJ...670L..89W)
Details on Acronym: GN
GN	(GOODS North)
*****	Avoid the usage of GN, prefer [PSD2006]
Origin	of the Acronym: L (2009ApJ...694.1517D)
Details on Acronym: GN-IRS
GN-IRS	(GOODS North, Spitzer/IRS)
*****	Avoid the usage of GN-IRS, prefer [MCA2009]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GN2009]
[GN2009]	(Ghosh+Narasimha, 2009)
Write:	<<[GN2009] lens>> <<[GN2009] image A>>
N:	1+2
Object:	G (SIMBAD class: Galaxy)
Note:	SDSS observations. Einstein Ring system of SDSS J091949.16+342304.0.
Ref:	=2009ApJ...692..694G
by	GHOSH K.K. , NARASIMHA D.
	Astrophys. J., 692, 694-701 (2009)
	A quasi-stellar object plus host system lensed into a 6'' Einstein ring by a low-redshift galaxy.
o	Text: <[GN2009] lens> N=1. Fig. 2, Text: <[GN2009] image A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GNA
GNA	(G, North, field A)
Write:	<<GNA NN>>
N:	80
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Anglo Australian Redshift Survey (AARS). See also GNB, GSA, GSAN, GSD, GSF
Ref:	=1986MNRAS.221..233P
by	PETERSON B.A. , ELLIS R.S., EFSTATHIOU G., SHANKS T., BEAN A.J., FONG R., ZEN-LONG Z.
	Mon. Not. R. Astron. Soc., 221, 233-255 (1986)
	A complete galaxy redshift sample - III. Methods and catalogue.
o	Table 3: <GSA NNNA> N=140 among (Nos 1-137), <GSAN N> (Nos 1-5), <GSD NNN> N=128 among (Nos 1-179), <GSF NNN> N=78 among (Nos 1-100), <GNA NN> N=80 among (Nos 1-81), <GNB NN> N=94 among (Nos 1-95)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GNB
GNB	(G, North, field B)
Write:	<<GNB NN>>
N:	94
Object:	G (SIMBAD class: Galaxy)
Note:	Anglo Australian Redshift Survey (AARS). See also GNA, GSA, GSAN, GSD, GSF
Ref:	=1986MNRAS.221..233P
by	PETERSON B.A. , ELLIS R.S., EFSTATHIOU G., SHANKS T., BEAN A.J., FONG R., ZEN-LONG Z.
	Mon. Not. R. Astron. Soc., 221, 233-255 (1986)
	A complete galaxy redshift sample - III. Methods and catalogue.
o	Table 3: <GSA NNNA> N=140 among (Nos 1-137), <GSAN N> (Nos 1-5), <GSD NNN> N=128 among (Nos 1-179), <GSF NNN> N=78 among (Nos 1-100), <GNA NN> N=80 among (Nos 1-81), <GNB NN> N=94 among (Nos 1-95)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GNC2005]
[GNC2005]	(Gosset+Naze+Claeskens+, 2005)
Write:	<<[GNC2005] NN>>
N:	33
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of the field of WR 40.
Ref:	=2005A&A...429..685G
by	GOSSET E. , NAZE Y., CLAESKENS J.-F., RAUW G., VREUX J.-M., SANA H.
	Astron. Astrophys., 429, 685-704 (2005)
	An XMM-Newton look at the Wolf-Rayet star WR 40. The star itself, its nebula and its neighbours.
o	Fig.8, Table 5: <[GNC2005] NN> (Nos 1-33).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GND2005]
[GND2005]	(Gerke+Newman+Davis+, 2005)
Write:	<<[GND2005] JHHMMSS+DDMMSS>>
N:	153
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	DEEP2 galaxy redshift survey: identification of groups of galaxies in redshift space.
Ref:	=2005ApJ...625....6G
by	GERKE B.F. , NEWMAN J.A., DAVIS M., MARINONI C., YAN R., COIL A.L., CONROY C., COOPER M.C., FABER S.M., FINKBEINER D.P., GUHATHAKURTA P., KAISER N., KOO D.C., PHILLIPS A.C., WEINER B.J., WILLMER C.N.A.
	Astrophys. J., 625, 6-22 (2005)
	The DEEP2 Galaxy Redshift Survey: first results on galaxy groups.
o	Table 3: <[GND2005] JHHMMSS+DDMMSS> N=153.
=E=	Catalogue in electronic form as J/ApJ/625/6
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GND2012]
[GND2012]	(Gerke+Newman+Davis+, 2012)
Write:	<<[GND2012] NNNN>>
N:	2460
Object:	Poss. Group of G (SIMBAD class: GroupG_Candidate = Group of Galaxies Candidate)
Note:	Public catalog of N=2460 galaxy groups constructed from the spectroscopic sample of galaxies in the fourth data release from the Deep Extragalactic Evolutionary Probe 2 (DEEP2) Galaxy Redshift Survey. This work updates and expands the group-finding efforts of Gerke et al., 2005ApJ...625....6G (see [GND2005]).
Ref:	=2012ApJ...751...50G
by	GERKE B.F. , NEWMAN J.A., DAVIS M., COIL A.L., COOPER M.C., DUTTON A.A., FABER S.M., GUHATHAKURTA P., KONIDARIS N., KOO D.C., LIN L., NOESKE K., PHILLIPS A.C., ROSARIO D.J., WEINER B.J., WILLMER C.N.A., YAN R.
	Astrophys. J., 751, 50 (2012)
	The DEEP2 Galaxy Redshift Survey: the Voronoi-Delaunay method catalog of galaxy groups.
o	Table 3: <[GND2012] NNNN> N=2460 among (Nos 1-2500).
=E=	Catalogue in electronic form as J/ApJ/751/50
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GNG92]
[GNG92]	(Garnavich+Noriega-Crespo+Green, 1992)= (G)
Write:	<<[GNG92] NNA>>
N:	34
Object:	Em. Obj. (SIMBAD class: PartofCloud = Part of Cloud)
Note:	Table 2: Emission objects in LDN 1551, (Nos 1-2, 3A-3C, 4A-4H, 5-6, 7A, 8-25). (No. 26) added in 1998AJ....116..845L
in source:	LDN 1551
Ref:	=1992RMxAA..24...99G
by	GARNAVICH P.M. , NORIEGA-CRESPO A., GREEN P.J.
	Rev. Mex. Astron. Astrofis., 24, 99-107 (1992)
	Wide field imaging of the star forming region Lynds 1551.
o	Table 1: <[GH90b] NNW> Nos 10W and 10E. Table 2: <[GNG92] NNA> (Nos 1-25), N=34
Ref:	=1998AJ....116..845L
by	LOPEZ R. , ROSADO M., RIERA A., NORIEGA-CRESPO A., RAGA A.C., ESTALELLA R., ANGLADA G., LE COARER E., LANGARICA R., TINOCO S., CANTO J.
	Astron. J., 116, 845-853 (1998)
	HH 262: the red lobe of the L1551 IRS 5 outflow.
o	Table 3, Fig.1: <[GNG92] NN> (No. 26) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GNH
GNH	(G, North, field H)
Write:	<<GNH NNN>>
N:	106
Object:	G (SIMBAD class: Galaxy)
Ref:	=1989MNRAS.236..207M
by	METCALFE N. , FONG R., SHANKS T., KILKENNY D.
	Mon. Not. R. Astron. Soc., 236, 207-234 (1989)
	An extended galaxy redshift survey - I. The catalogue.
o	<GNH NNN> (Nos 1-106), <GNX NNN> (Nos 1-113), <GNY NN> (Nos 1-91), <GNZ NNN> (Nos 1-130), <GSG NNN> (Nos 1-159), <GSI NNN> (Nos 1-136), <GSM NNN> (Nos 1-130), <GSN NNN> (Nos 1-195), <GSP NN> (Nos 1-74)
=E=	Catalogue in electronic form as J/MNRAS/236/207
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GNM2016]
[GNM2016]	(Geach+Narayanan+Matsuda+, 2016)
Write:	<<[GNM2016] SSA22-LAB01 ALMA a>> <<[GNM2016] SSA22-LAB01 ALMA a+b>> <<[GNM2016] S1>>
N:	3+1+1
Object:	(smm) + (UV) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	ALMA 850µm, HST STIS, and Keck I MOSFIRE observations of N=3 submillimeter components, and N=1 faint companion, in the Lyα blob [TSK2001] LAB 1. See also [UMT2017].
in source:	[TSK2001] LAB 1 = [MYH2004] LAB 1
Ref:	=2016ApJ...832...37G
by	GEACH J.E. , NARAYANAN D., MATSUDA Y., HAYES M., MAS-RIBAS L., DIJKSTRA M., STEIDEL C.C., CHAPMAN S.C., FELDMANN R., AVISON A., AGERTZ O., AO Y., BIRKINSHAW M., BREMER M.N., CLEMENTS D.L., DANNERBAUER H., FARRAH D., HARRISON C.M., KUBO M., MICHALOWSKI M.J., SCOTT D., SMITH D.J.B., SPAANS M., SIMPSON J.M., SWINBANK A.M., TANIGUCHI Y., VAN DER WERF P., VERMA A., YAMADA T.
	Astrophys. J., 832, 37-37 (2016)
	ALMA observations of Lyα Blob 1: halo substructure illuminated from within.
o	Fig. 1, Table 1: <[GNM2016] SSA22-LAB01 ALMA a> (Nos a-c), <[GNM2016] SSA22-LAB01 ALMA a+b> N=1, <[GNM2016] S1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GNO
GNO	(Group No.)
*****	Avoid the usage of GNO, prefer [HG82]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GNO2008]
[GNO2008]	(Gal-Yam+Nakar+Ofek+, 2008)
Write:	<<[GNO2008] YYMMSS-{G\|N}N>> <<[GNO2008] YYMMSS-M>> <<[GNO2008] YYMMSS Host>>
N:	12+1+2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Optical photometry and spectroscopy of galaxies in the fields of short-hard gamma-ray bursts.
Ref:	=2008ApJ...686..408G
by	GAL-YAM A. , NAKAR E., OFEK E.O., CENKO S.B., KULKARNI S.R., SODERBERG A.M., HARRISON F., FOX D.B., PRICE P.A., PENPRASE B.E., FRAIL D.A., ATTEIA J.L., BERGER E., GLADDERS M., MULCHAEY J.
	Astrophys. J., 686, 408-416 (2008)
	New imaging and spectroscopy of the locations of several short-hard γ-ray bursts.
o	Table 2: <[GNO2008] YYMMSS-AN>, <[GNO2008] YYMMSS-M>, N=12+1. Table 3: <[GNO2008] YYMMSS Host> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GNR2008]
[GNR2008]	(Gatti+Natta+Randich+, 2008)
Write:	<<[GNR2008] NN>>
N:	35
Object:	TTau* (SIMBAD class: TTauri* = T Tauri Star)
Stat:	is completely incorporated in Simbad
Note:	NTT SOFI NIR observations of N=35 T Tauri stars in the sig Ori Cluster
in source:	NAME sig Ori Cluster
Ref:	=2008A&A...481..423G
by	GATTI T. , NATTA A., RANDICH S., TESTI L., SACCO G.
	Astron. Astrophys., 481, 423-432 (2008)
	Accretion properties of T Tauri stars in σ Orionis.
o	Table 1: <[GNR2008] NN> (Nos 1-35).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GNRB
GNRB	(Garnavich+Noriega-Crespo+Raga+Bohm)
Write:	<<GNRB HH 110 NN>>
N:	17
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Map in Fig.1
in source:	HH 110
Ref:	=1997ApJ...490..752G
by	GARNAVICH P.M. , NORIEGA-CRESPO A., RAGA A.C., BOEHM K.
	Astrophys. J., 490, 752-757 (1997)
	Highly collimated molecular hydrogen jets near IRAS 05487+0255: near-infrared imaging and spectroscopy.
o	Table 2: IRS 1 and 2 = [DME94] HH 110 IRS 1 and 2, star 1 = [RO91] 1
o	Table 2: <GNRB HH 110 NN> (Nos 1-17)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GNS
GNS	(GOODS NICMOS Survey)
Write:	<<GNS NNNN>>
N:	8298
Object:	G (SIMBAD class: Galaxy)
Note:	HST NICMOS observations of N=8298 galaxies, as part of the GOODS NICMOS Survey.
Ref:	=2011MNRAS.413...80C
by	CONSELICE C.J. , BLUCK A.F.L., BUITRAGO F., BAUER A.E., GRUTZBAUCH R., BOUWENS R.J., BEVAN S., MORTLOCK A., DICKINSON M., DADDI E., YAN H., SCOTT D., CHAPMAN S.C., CHARY R.-R., FERGUSON H.C., GIAVALISCO M., GROGIN N., ILLINGWORTH G., JOGEE S., KOEKEMOER A.M., LUCAS R.A., MOBASHER B., MOUSTAKAS L., PAPOVICH C., RAVINDRANATH S., SIANA B., TEPLITZ H., TRUJILLO I., URRY M., WEINZIRL T.
	Mon. Not. R. Astron. Soc., 413, 80-100 (2011)
	The Hubble Space Telescope GOODS NICMOS Survey: overview and the evolution of massive galaxies at 1.5< z< 3.
o	<GNS NNNN> (Nos 1-8298).
=E=	Catalogue in electronic form as J/MNRAS/413/80
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GNS2018]
[GNS2018]	(Gomez+Niccolini+Suarez+, 2018)
Write:	<<[GNS2018] A>>
N:	2
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 6 (1.3mm) and Band 7 (0.85mm) observations of N=2 continuum sources in the field of IRAS 15103-5754.
Ref:	=2018MNRAS.480.4991G
by	GOMEZ J.F. , NICCOLINI G., SUAREZ O., MIRANDA L.F., RIZZO J.R., USCANGA L., GREEN J.A., DE GREGORIO-MONSALVO I.
	Mon. Not. R. Astron. Soc., 480, 4991-5009 (2018)
	ALMA imaging of the nascent planetary nebula IRAS 15103-5754.
o	Fig. 1, Table 2: <[GNS2018] A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GNT
GNT	(Gaia Nuclear Transient)
*****	Avoid the usage of GNT, prefer [KJH2018]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GNX
GNX	(G, North, field X)
Write:	<<GNX NNN>>
N:	113
Object:	G (SIMBAD class: Galaxy)
Ref:	=1989MNRAS.236..207M
by	METCALFE N. , FONG R., SHANKS T., KILKENNY D.
	Mon. Not. R. Astron. Soc., 236, 207-234 (1989)
	An extended galaxy redshift survey - I. The catalogue.
o	<GNH NNN> (Nos 1-106), <GNX NNN> (Nos 1-113), <GNY NN> (Nos 1-91), <GNZ NNN> (Nos 1-130), <GSG NNN> (Nos 1-159), <GSI NNN> (Nos 1-136), <GSM NNN> (Nos 1-130), <GSN NNN> (Nos 1-195), <GSP NN> (Nos 1-74)
=E=	Catalogue in electronic form as J/MNRAS/236/207
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GNY
GNY	(G, North, field Y)
Write:	<<GNY NN>>
N:	91
Object:	G (SIMBAD class: Galaxy)
Ref:	=1989MNRAS.236..207M
by	METCALFE N. , FONG R., SHANKS T., KILKENNY D.
	Mon. Not. R. Astron. Soc., 236, 207-234 (1989)
	An extended galaxy redshift survey - I. The catalogue.
o	<GNH NNN> (Nos 1-106), <GNX NNN> (Nos 1-113), <GNY NN> (Nos 1-91), <GNZ NNN> (Nos 1-130), <GSG NNN> (Nos 1-159), <GSI NNN> (Nos 1-136), <GSM NNN> (Nos 1-130), <GSN NNN> (Nos 1-195), <GSP NN> (Nos 1-74)
=E=	Catalogue in electronic form as J/MNRAS/236/207
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GNZ
GNZ	(G, North, field Z)
Write:	<<GNZ NNN>>
N:	130
Object:	G (SIMBAD class: Galaxy)
Ref:	=1989MNRAS.236..207M
by	METCALFE N. , FONG R., SHANKS T., KILKENNY D.
	Mon. Not. R. Astron. Soc., 236, 207-234 (1989)
	An extended galaxy redshift survey - I. The catalogue.
o	<GNH NNN> (Nos 1-106), <GNX NNN> (Nos 1-113), <GNY NN> (Nos 1-91), <GNZ NNN> (Nos 1-130), <GSG NNN> (Nos 1-159), <GSI NNN> (Nos 1-136), <GSM NNN> (Nos 1-130), <GSN NNN> (Nos 1-195), <GSP NN> (Nos 1-74)
=E=	Catalogue in electronic form as J/MNRAS/236/207
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GO
GO	(Gratton+Ortolani)
Write:	<<GO NNNN>>
N:	392
Object:	* (SIMBAD class: Star)
Note:	In the format first digit 'N' stands for the two frames 1 or 2. Format with always 4 digits.
in source:	C 0435-589
Ref:	=1987A&AS...71..131G
by	GRATTON R.S. , ORTOLANI S.
	Astron. Astrophys., Suppl. Ser., 71, 131-146 (1987)
	Deep photometry of globular clusters. X. The cluster GlC 0435-59 in Reticulum.
o	GlC 0435-59 = C 0435-589
o	<GO NNNN> N=392, format with always 4 digits
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GO2007a]
[GO2007a]	(Galfalk+Olofsson, 2007)
*****	Avoid the usage of [GO2007a], prefer [GO2008]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GO2007b]
[GO2007b]	(Galfalk+Olofsson, 2007)
Write:	<<[GO2007b] IR Na>>
N:	7+20
Object:	H2 (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	NOT 2.12mu.m H2 narrow-band observations of Barnard 335. See also [H98b].
in source:	Barnard 335
Ref:	=2007A&A...475..281G
by	GALFALK M. , OLOFSSON G.
	Astron. Astrophys., 475, 281-300 (2007)
	Herbig-Haro flows in B335.
o	Figs 1, 2, Table 2: <[GO2007b] IR Na> (Nos 1-8, 6 missing, 4a-4b, 7a-7c, 8a-8o).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GO2008]
[GO2008]	(Galfalk Olofsson, 2008)= ([GO2007a])
Write:	<<[GO2008] NNN>> <<[GO2008] L1641N-NNN>> (not recognised by Simbad, but found in literature)
N:	213
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Note:	ISO ISOCAM, Spitzer IRAC and NOT NOTcam-AFOSC-SIRCA observations of LDN 1641N.
in source:	LDN 1641:LDN 1641N = LDN 1641N
Ref:	=2008A&A...489.1409G
by	GALFALK M. , OLOFSSON G.
	Astron. Astrophys., 489, 1409-1439 (2008)
	A detailed study of the L1641N star formation region.
o	Table 11: <[GO2008] NNN> N=213 among (Nos 1-216).
=E=	Catalogue in electronic form as J/A+A/489/1409
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GO75]
[GO75]	(Gunn+Oke, 1975) (Not yet in Simbad)
Write:	<<[GO75] NN>>
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	N=28 large-redshift bright galaxies in 26 clusters.
Ref:	=1975ApJ...195..255G
by	GUNN J.E. , OKE J.B.
	Astrophys. J., 195, 255-268 (1975)
	Spectrophotometry of faint cluster galaxies and the Hubble diagram: an approach to cosmology.
o	Table 1: <[GO75] NN> (Nos 1-28).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GOA94]
[GOA94]	(Gyulbudaghian+Oganian+Akhverdian, 1994)
*****	Avoid the usage of [GOA94], prefer [GA90]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GOALS
GOALS	(Great Observatories All-sky LIRG Survey)
Write:	<<GOALS JHHMMSS.ss+DDMMSS.s>>
N:	3+119
Object:	Poss. Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	The Great Observatories All-sky LIRG Survey (GOALS) is combining imaging and spectroscopic data from NASA's Spitzer, Hubble, Chandra and GALEX space-borne observatories (description in Armus et al. 2009PASP..121..559A).
Ref:	=2011A&A...528A.137I
by	IWASAWA K. , MAZZARELLA J.M., SURACE J.A., SANDERS D.B., ARMUS L., EVANS A.S., HOWELL J.H., KOMOSSA S., PETRIC A., TENG S.H., U V., VEILLEUX S.
	Astron. Astrophys., 528A, 137-137 (2011)
	The location of an active nucleus and a shadow of a tidal tail in the ULIRG Mrk 273.
o	Paragr. 3.1: <[IMS2011] CSCN> (Nos CSC1-CSC3) = <GOALS JHHMMSS.ss+DDMMSS.s> N=3.
Ref:	=2012AJ....144..125M
by	MAZZARELLA J.M. , IWASAWA K., VAVILKIN T., ARMUS L., KIM D.-C., BOTHUN G., EVANS A.S., SPOON H.W.W., HAAN S., HOWELL J.H., LORD S., MARSHALL J.A., ISHIDA C.M., XU C.K., PETRIC A., SANDERS D.B., SURACE J.A., APPLETON P., CHAN B.H.P., FRAYER D.T., INAMI H., KHACHIKIAN E.Y., MADORE B.F., PRIVON G.C., STURM E., U V., VEILLEUX S.
	Astron. J., 144, 125 (2012)
	Investigation of dual active nuclei, outflows, shock-heated gas, and young star clusters in Markarian 266.
o	Table 15: <[MIV2012] Mrk 266 SCNNN> (Nos 1-119) = <GOALS JHHMMSS.ss+DDMMSS.s> N=119.
=E=	Catalogue in electronic form as <J/AJ/144/125/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GOALS
GOALS	(Great Observatories All-sky LIRG Survey)
*****	Avoid the usage of GOALS, prefer [HAM2010]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GOK2004]
[GOK2004]	(Galfalk+Olofsson+Kaas+, 2004)
Write:	<<[GOK2004] NN>>
N:	96
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	ISOCAM survey of LDN 1551. Additional Halpha, BVIK observations with the NOT telescope, Canary Islands. Identification of 15 new YSO candidates.
in source:	LDN 1551
Ref:	=2004A&A...420..945G
by	GALFALK M. , OLOFSSON G., KAAS A.A., OLOFSSON S., BONTEMPS S., NORDH L., ABERGEL A., ANDRE P., BOULANGER F., BURGDORF M., CASALI M.M., CESARSKY C.J., DAVIES J., FALGARONE E., MONTMERLE T., PERAULT M., PERSI P., PRUSTI T., PUGET J.L., SIBILLE F.
	Astron. Astrophys., 420, 945-955 (2004)
	ISOCAM observations of the L1551 star formation region.
o	Table 2: <[GOK2004] NN> (Nos 1-96).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Gomez
Gomez	(Gomez+)
*****	Avoid the usage of Gomez, prefer [GHK93]
Origin	of the Acronym: L (1998AJ....115.2074B)
Details on Acronym: GOODS
GOODS	(Great Observatories Origins Deep Survey)= (GDS) = (GOODSN)
Write:	<<GOODS JHHMMSS.ss+DDMMSS.s>>
N:	32048+29599
Object:	G (SIMBAD class: Galaxy)
Note:	Observations of the GOODS-North and -South fields. The initial HST GOODS catalogues are described in 2004ApJ...600L..93G.
in source:	NAME GOODS North Field
in source:	NAME GOODS South Field
Ref:	=2004ApJ...600L..93G
by	GIAVALISCO M. , FERGUSON H.C., KOEKEMOER A.M., DICKINSON M., ALEXANDER D.M., BAUER F.E., BERGERON J., BIAGETTI C., BRANDT W.N., CASERTANO S., CESARSKY C., CHATZICHRISTOU E., CONSELICE C., CRISTIANI S., DA COSTA L., DAHLEN T., DE MELLO D., EISENHARDT P., ERBEN T., FALL S.M., FASSNACHT C., FOSBURY R., FRUCHTER A., GARDNER J.P., GROGIN N., HOOK R.N., HORNSCHEMEIER A.E., IDZI R., JOGEE S., KRETCHMER C., LAIDLER V., LEE K.S., LIVIO M., LUCAS R., MADAU P., MOBASHER B., MOUSTAKAS L.A., NONINO M., PADOVANI P., PAPOVICH C., PARK Y., RAVINDRANATH S., RENZINI A., RICHARDSON M., RIESS A., ROSATI P., SCHIRMER M., SCHREIER E., SOMERVILLE R.S., SPINRAD H., STERN D., STIAVELLI M., STROLGER L., URRY C.M., VANDAME B., WILLIAMS R., WOLF C.
	Astrophys. J., 600, 93-98 (2004)
	The Great Observatories Origins Deep Survey: initial results from optical and near-infrared imaging.
o	Catalog: <GOODS JHHMMSS.ss+DDMMSS.s> N=32048+29599.
=E=	Catalogue in electronic form as II/261
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GOODS 850
GOODS 850	(GOODS, 850mu.m)
*****	Avoid the usage of GOODS 850, prefer [WCB2004]
Origin	of the Acronym: L (2007ApJ...670L..89W)
Details on Acronym: GOODS-MUSIC
GOODS-MUSIC	(GOODS, Multiwavelength Southern IR Catalog)= (CDFS)
Write:	<<GOODS-MUSIC NNNNN>>
N:	18657
Object:	G (SIMBAD class: Galaxy)
Note:	Multiwavelength catalogue of the large and deep area in the GOODS Southern Field covered by the deep near-IR observations obtained with the ESO VLT. The analysis takes into account data from HST ACS, VLT EIS, ISAAC and VIMOS, and Spitzer IRAC.
in source:	NAME GOODS South Field
Ref:	=2006A&A...449..951G
by	GRAZIAN A. , FONTANA A., DE SANTIS C., NONINO M., SALIMBENI S., GIALLONGO E., CRISTIANI S., GALLOZZI S., VANZELLA E.
	Astron. Astrophys., 449, 951-968 (2006)
	The GOODS-MUSIC sample: a multicolour catalog of near-IR selected galaxies in the GOODS-South field.
o	Table 5: <GOODS-MUSIC NNNNN> (Nos 1-18296).
Ref:	=2009A&A...504..751S
by	SANTINI P. , FONTANA A., GRAZIAN A., SALIMBENI S., FIORE F., FONTANOT F., BOUTSIA K., CASTELLANO M., CRISTIANI S., DE SANTIS C., GALLOZZI S., GIALLONGO E., MENCI N., NONINO M., PARIS D., PENTERICCI L., VANZELLA E.
	Astron. Astrophys., 504, 751-767 (2009)
	Star formation and mass assembly in high redshift galaxies.
o	catalog: <GOODS-MUSIC NNNNN> N=18657 among (Nos 1-70542).
=E=	Catalogue in electronic form as J/A+A/449/951
=E=	Catalogue in electronic form as J/A+A/504/751
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GOODSN
GOODSN	(Great Observatories Origins Deep Survey, North)
*****	Avoid the usage of GOODSN, prefer GOODS
Origin	of the Acronym: L (2007AJ....134...77M)
Details on Acronym: Gopal
Gopal	(Gopal-Krishna+)= (GPS)
Write:	<<Gopal HHMM+DDd>>
N:	129
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	The authors use the acronym GPS for 'Gigahertz Peaked-Spectrum'.
Ref:	=1983A&A...123..107G
by	GOPAL-KRISHNA , PATNAIK A.R., STEPPE H.
	Astron. Astrophys., 123, 107-110 (1983)
	A sample of 25 extragalactic radio sources having a spectrum peaked around 1 GHz.
o	<Gopal HHMM+DDd>, N=25
Ref:	=1985A&A...152...38S
by	SPOELSTRA T.A.T. , PATNAIK A.R., GOPAL-KRISHNA
	Astron. Astrophys., 152, 38-41 (1985)
	A sample of 25 extragalactic radio sources having a spectrum peaked around 1 GHz (list 2).
o	<Gopal HHMM+DDd> N=25
Ref:	=1993A&A...271..101G
by	GOPAL-KRISHNA , SPOELSTRA T.A.T.
	Astron. Astrophys., 271, 101-103 (1993)
	A sample of gigahertz-peaked-spectrum radio sources: List 3.
o	<Gopal HHMM+DDd> N=10
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GOR2018]
[GOR2018]	(Gorski+Ott+Rand+, 2018) (Not yet in Simbad)
Write:	<<[GOR2018] IC 342 AN>> <<[GOR2018] IC 342 A'N>> <<[GOR2018] {NGC} {6946\|2146} AR>>
N:	5+3+3
Object:	Cloud (SIMBAD class: MolCld = Molecular Cloud)
Note:	VLA NH3 line observations in the central kpc of IC 342, NGC 6946 and NGC 2146.
in source:	IC 342
in source:	NGC 6946
in source:	NGC 2146
Ref:	=2018ApJ...856..134G
by	GORSKI M. , OTT J., RAND R., MEIER D.S., MOMJIAN E., SCHINNERER E.
	Astrophys. J., 856, 134-134 (2018)
	Survey of Water and Ammonia in Nearby galaxies (SWAN): resolved ammonia thermometry and Water and methanol masers in IC 342, NGC 6946, and NGC 2146.
o	Table 4: <[GOR2018] IC 342 AN> (Nos A1-A2, C4-C5, E3), <[GOR2018] IC 342 A'N> (Nos D'1-D'3), <[GOR2018] NGC 6946 AR> (No. AI), <[GOR2018] NGC 2146 AR> (Nos AI-AII).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GOS
GOS	(Galactic O Star)
Write:	<<GOS GLLL.ll+BB.bb NN>>
N:	139+378+309+142
Object:	0 * (SIMBAD class: Star)
Note:	The Galactic O-Star Spectroscopic Survey (GOSSS) is a long-term project that is obtaining homogeneous, high SNR, R∼2500, blueviolet spectra of a large number (1000+) of O stars in the Milky Way. The Galactic O-Star Catalog (GOSC) is accessible at: https://gosc.cab.inta-csic.es/
Ref:	=2004ApJS..151..103M
by	MAIZ-APELLANIZ J. , WALBORN N.R., GALUE H.A., WEI L.H.
	Astrophys. J., Suppl. Ser., 151, 103-148 (2004)
	A galactic O star catalog.
o	Table 1: <GOS GLLL.ll+BB.bb NN> N=378.
Ref:	=2011ApJS..193...24S
by	SOTA A. , MAIZ-APELLANIZ J., WALBORN N.R., ALFARO E.J., BARBA R.H., MORRELL N.I., GAMEN R.C., ARIAS J.I.
	Astrophys. J., Suppl. Ser., 193, 24 (2011)
	The Galactic O-Star Spectroscopic Survey. I. Classification system and bright northern stars in the blue-violet at R ~ 2500.
o	<GOS GLLL.ll+BB.bb NN> N=139.
Ref:	=2014ApJS..211...10S
by	SOTA A. , MAIZ APELLANIZ J., MORRELL N.I., BARBA R.H., WALBORN N.R., GAMEN R.C., ARIAS J.I., ALFARO E.J.
	Astrophys. J., Suppl. Ser., 211, 10 (2014)
	The Galactic O-Star Spectroscopic Survey (GOSSS). II. Bright southern stars.
o	<GOS GLLL.ll+BB.bb NN> N=309.
Ref:	=2016ApJS..224....4M
by	MAIZ-APELLANIZ J. , SOTA A., ARIAS J.I., BARBA R.H., WALBORN N.R., SIMON-DIAZ S., NEGUERUELA I., MARCO A., LEAO J.R.S., HERRERO A., GAMEN R.C., ALFARO E.J.
	Astrophys. J., Suppl. Ser., 224, 4 (2016)
	The Galactic O-star Spectroscopic Survey (GOSSS). III. 142 additional O-type systems.
o	Table 5: <GOS GLLL.ll+BB.bb NN> N=142 added.
=E=	Catalogue in electronic form as V/116
=E=	Catalogue in electronic form as III/274
=E=	Catalogue in electronic form as <J/ApJS/211/10/>
=E=	Catalogue in electronic form as <J/ApJS/224/4/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GOS2002]
[GOS2002]	(Gal-Yam+Ofek+Shemmer, 2002)
Write:	<<[GOS2002] NN>>
N:	10
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=10 reference stars in the field of SN 2002AP.
Ref:	=2002MNRAS.332L..73G
by	GAL-YAM A. , OFEK E.O., SHEMMER O.
	Mon. Not. R. Astron. Soc., 332, 73-77 (2002)
	Supernova 2002ap: the first month.
o	Table 1: <[GOS2002] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GOS97]
[GOS97]	(Goldschmidt+Oliver+Serjeant+, 1997)= (IC)
Write:	<<[GOS97] JHHMMSS.s+DDMMSS>>
N:	49
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	ISO CAM observations. See also ISOHDF, [ACE99], [DPC99]
in source:	NAME HDFN
Ref:	=1997MNRAS.289..465G
by	GOLDSCHMIDT P. , OLIVER S.J., SERJEANT S.B.G., BAKER A., EATON N., EFSTATHIOU A., GRUPPIONI C., MANN R.G., MOBASHER B., ROWAN-ROBINSON M., SUMNER T.J., DANESE L., ELBAZ D., FRANCESCHINI A., EGAMI E., KONTIZAS M., LAWRENCE A., McMAHON R., NORGAARD-NIELSEN H.U., PEREZ-FOURNON I., GONZALEZ-SERRANO J.I.
	Mon. Not. R. Astron. Soc., 289, 465-470 (1997)
	Observations of the Hubble Deep Field with the Infrared Space Observatory - II. Source detection and photometry.
o	Tables 2, 3, 5, 6: <[GOS97] JHHMMSS.s+DDMMSS> = <ISOHDF JHHMMSS.s+DDMMSS> N=49.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Goy
Goy	(Goy)
Write:	<<Goy NNN>>
N:	971
Object:	O * (SIMBAD class: Star)
Ref:	=1980A&AS...42...91G
by	GOY G.
	Astron. Astrophys., Suppl. Ser., 42, 91-102 (1980)
	Catalogue general d'etoiles de type O. Donnees spectroscopiques et photometriques. Bande magnetique et listage.
o	in description des colonnes WALKER 1956ApJS....2..365W instead of ApJ.2 3.365, in bibliographie ANDREWS 1968MmRAS..72...35A instead MNRAS
o	<Goy NNN> (Nos 1-971)
=E=	Catalogue in electronic form as II/76
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Gp
Gp	(Grebenev+, PSPC)
*****	Avoid the usage of Gp, prefer [GFJ95]
Origin	of the Acronym: L (2002ApJ...576..708S)
Details on Acronym: GP
GP	(Godwin+Peach)
Write:	<<GP NNN>>
N:	923
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	map. See also [AP74], [AGP75], BGP, [GP82]
in source:	Coma Cluster = ACO 1656
Ref:	=1977MNRAS.181..323G
by	GODWIN J.G. , PEACH J.V.
	Mon. Not. R. Astron. Soc., 181, 323-337 (1977)
	Studies of rich clusters of galaxies. IV. Photometry of the Coma cluster.
o	Table 1: <GP NNN> (Nos 1-923)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: GP
GP	(Glass+Penston)
*****	Avoid the usage of GP, prefer [GP75]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: GP
GP	(Godwin+Peach)
*****	Avoid the usage of GP, prefer [GP82]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GP2003]
[GP2003]	(Gusev+Park, 2003) (Not yet in Simbad)
Write:	<<[GP2003] NNa>>
N:	34
Object:	Star Forming Region (SIMBAD class: Region = Region defined in the Sky)
Note:	Structure of the galaxy NGC 2336. Table 5: star formation regions.
in source:	NGC 2336
Ref:	=2003A&A...410..117G
by	GUSEV A.S. , PARK M.-G.
	Astron. Astrophys., 410, 117-129 (2003)
	Structure and stellar population of ringed barred galaxy NGC 2336.
o	Table 5: <[GP2003] NNa> (Nos 1-26, 27a-27e, 28-30).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GP2008]
[GP2008]	(Ghosh+Punsly, 2008) (Not yet in Simbad)
Write:	<<[GP2008] 1WGA JHHMM.m+DDMM N>>
N:	4+6+5
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT detections in 3 BALQSOs.
in source:	1WGA J0232.0+0021
in source:	1WGA J1019.0+4502
in source:	1WGA J1322.0+1410
Ref:	=2008ApJ...674L..69G
by	GHOSH K.K. , PUNSLY B.
	Astrophys. J., 674L, 69-72 (2008)
	The discovery of soft X-ray-loud broad absorption line quasars.
o	Paragr.1: IRAS 07598+059 not identified. Paragr.2: 1WGA J1019.7+4502 = SDSS J101942.92+450239.4 (not SDSS J101949.75+450256.0).
o	Fig.2, Table 2: <[GP2008] 1WGA J0232.3+0021 N> (Nos 1-4), <[GP2008] 1WGA J1019.7+4502 N> (Nos 1-6), <[GP2008] 1WGA J1322.4+1410 N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GP75]
[GP75]	(Glass+Penston, 1975)= (GP)
Write:	<<[GP75] R CrA a>> <<[GP75] R CrA aN>>
N:	26+12
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Finding chart.
in source:	NAME R CrA Cloud
Ref:	=1975MNRAS.172..227G
by	GLASS I.S. , PENSTON M.V.
	Mon. Not. R. Astron. Soc., 172, 227-233 (1975)
	Infrared photometry in the R CrA association.
o	Table I: <[GP75] R CrA aN> (Nos a-z a2-l2) N=26+12
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GP82]
[GP82]	(Godwin+Peach, 1982)= (GP)
Write:	<<[GP82] NNNN>>
N:	1561
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	See also [AP74], [AGP75], BGP, GP
in source:	ACO 1367
Ref:	=1982MNRAS.200..733G
by	GODWIN J.G. , PEACH J.V.
	Mon. Not. R. Astron. Soc., 200, 733-746 (1982)
	Photometry of the cluster of galaxies A 1367.
o	cata on microfiche MN 200/2
o	<[GP82] NNNN> (Nos 1-1561)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GP89]
[GP89]	(Gonzalez-Serrano+Perez-Fournon, 1989)
Write:	<<[GP89] HHMM+DD A>>
N:	1+2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	CCD images of elliptical galaxies: B2 0034+25 radio galaxy has a close companion 'B'. B2 2236+35 radio galaxy has two close neighbour galaxies 'B' and 'C'.
Ref:	=1989Ap&SS.156..121G
by	GONZALEZ-SERRANO J.I. , PEREZ-FOURNON I.
	Astrophys. Space Sci., 156, 121-125 (1989)
	Morphological properties of radio elliptical galaxies.
o	Text, Figs: <[GP89] 0034+25 A> (No. B). <[GP89] 2236+35 A> (Nos B, C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GP96]
[GP96]	(Gonzalez Delgado+Perez, 1996)= ([GP96a])
Write:	<<[GP96] NN>>
N:	33
Object:	HII (SIMBAD class: HIIReg = HII Region)
in source:	NGC 5347
Ref:	=1996MNRAS.280...53G
by	GONZALEZ-DELGADO R.M. , PEREZ E.
	Mon. Not. R. Astron. Soc., 280, 53-66 (1996)
	The emission-line knot in the Seyfert 2 galaxy NGC 5347.
o	Table 2: <[GP96] NN> (Nos 1-33)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GP96a]
[GP96a]	(Gonzalez Delgado+Perez, 1996)
*****	Avoid the usage of [GP96a], prefer [GP96]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GP96b]
[GP96b]	(Gonzalez Delgado+Perez, 1996) (Not yet in Simbad)
Write:	<<[GP96b] NGC NNNN NN>>
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	HII regions in the circumnuclear region in NGC 5953 and in the disc in NGC 5954.
in source:	NGC 5953
in source:	NGC 5954
Ref:	=1996MNRAS.281..781G
by	GONZALEZ-DELGADO R.M. , PEREZ E.
	Mon. Not. R. Astron. Soc., 281, 781-798 (1996)
	The circumnuclear region in the Seyfert 2 galaxy NGC 5953.
o	Table 2: <[GP96b] NGC 5953 NN> (Nos 1-11), <[GP96b] NGC 5954 NN> (Nos 1-25).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GP97]
[GP97]	(Gonzalez Delgado+Perez, 1997) (Not yet in Simbad)
Write:	<<[GP97] NN>>
N:	29
Object:	HII (SIMBAD class: HIIReg = HII Region)
in source:	NGC 3227
Ref:	=1997MNRAS.284..931G
by	GONZALEZ-DELGADO R.M. , PEREZ E.
	Mon. Not. R. Astron. Soc., 284, 931-945 (1997)
	The circumnuclear region in the Seyfert 1 galaxy NGC 3227.
o	Table 2: <[GP97] NN> (Nos 1-29)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GPA
GPA	(Galactic Plane A survey)= ([LMD2000b])
Write:	<<GPA LLL.ll+B.bb>>
N:	677
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Galactic Plane A survey: l = -15deg to 255deg, b = -5deg to +5deg, first images of galactic sources, HII regions, SNRs and transients. See also GPB. These observations used the NRAO/NASA Green Bank Earth Station to survey the sky simultaneously at these frequencies. These are the first results from the Galactic Plane (GP) survey observations, a program to monitor the sky at 8.35 and 14.35 GHz. The GP survey series is intended to detect short lived radio-sources. We present four independent observations of the galactic plane, combined to provide a set of reference images of the galactic plane. We compare the relative brightness of Cassiopeia A and Cygnus A and find the rate of decrease of Cassiopeia A is slower than previously reported. The first survey, GPA, covers 0.82 sr (6.5%) of the sky. A source list is presented for all sources brighter than 0.9Jy at 8.35GHz and also for all sources brighter than 2.5 Jy at 14.35 GHz.
Ref:	=2000AJ....119.2801L
by	LANGSTON G. , MINTER A., D'ADDARIO L., EBERHARDT K., KOSKI K., ZUBER J.
	Astron. J., 119, 2801-2827 (2000)
	The first galactic plane survey at 8.35 and 14.35 GHz.
o	Table 3: <GPA LLL.ll+B.bb> N=677.
=E=	Catalogue in electronic form as J/AJ/119/2801
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [GPA2005]
[GPA2005]	(Galliano+Pantin+Alloin+, 2005)
Write:	<<[GPA2005] WWN>>
N:	7+5
Object:	(Mid IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Mid-IR images of the central region of NGC 1068 with VISIR at the EOO VLT.
in source:	NGC 1068
Ref:	=2005MNRAS.363L...1G
by	GALLIANO E. , PANTIN E., ALLOIN D., LAGAGE P.O.
	Mon. Not. R. Astron. Soc., 363, 1-5 (2005)
	Mid-infrared imaging of NGC 1068 with VISIR at the Very Large Telescope.
o	Table 1: <[GPA2005] WWN> (Nos NE1-NE7, SW1-SW5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GPB
GPB	(Galactic Plane B survey) (Not yet in Simbad)
Write:	<<GPB GLLL.ll+B.bb>>
N:	about 600
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	In preparation. Galactic Plane B survey: l = -15deg to 255deg, b = -5deg to +5deg. Second images of galactic sources, HII regions, SNRs and transients. See also GPA.
Notes:	We present the second images of the galactic plane (\|b\| < 5deg, l = -15 deg to 255 deg) at 8.35 and 14.35 GHz. These observations used the NRAO/NASA Green Bank Earth Station to survey the sky simultaneously at these frequencies. These are the second results from the Galactic Plane (GP) survey observations, a program to monitor the sky at 8.35 and 14.35 GHz. The GP survey series is intended to detect short lived radio-sources.
Auth.:	LANGSTON G. National Radio Astronomy Observatory
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [GPB2005]
[GPB2005]	(Gaga+Plionis+Basilakos+, 2005)
Write:	<<[GPB2005] N>>
N:	8
Object:	(X) (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton 2dF survey: sample of 8 extended X-ray sources identified as candidate cluster of Galaxies.
Ref:	=2005MNRAS.363..811G
by	GAGA T. , PLIONIS M., BASILAKOS S., GEORGANTOPOULOS I., GEORGAKAKIS A.
	Mon. Not. R. Astron. Soc., 363, 811-817 (2005)
	The XMM-Newton/2dF survey - VIII. The extended X-ray sources.
o	Table 1: <[GPB2005] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPB2012]
[GPB2012]	(Ghosh+Prasad+Bharadwaj+, 2012)
Write:	<<[GPB2012] GMRT JHHMMSS.s+DDMMSS.s>>
N:	206
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	GMRT 150MHz observations of N=206 sources.
Ref:	=2012MNRAS.426.3295G
by	GHOSH A. , PRASAD J., BHARADWAJ S., ALI S.S., CHENGALUR J.N.
	Mon. Not. R. Astron. Soc., 426, 3295-3314 (2012)
	Characterizing foreground for redshifted 21cm radiation: 150MHz Giant Metrewave Radio Telescope observations.
o	Table A1: <[GPB2012] GMRT JHHMMSS.s+DDMMSS.s> N=206.
=E=	Catalogue in electronic form as <J/MNRAS/426/3295/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPC2018]
[GPC2018]	(Galametz+Pentericci+Castellano+, 2018)
Write:	<<[GPC2018] CN>> <<[GPC2018] UNN>> <<[GPC2018] U1N>> <<[GPC2018] UKIDSSNNNNNN>>
N:	9+25+1+379
Object:	Poss. Cluster of G + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT VIMOS observations of N=35 galaxy cluster candidates and N=379 galaxies in the UKIDSS UDS field. Use of CANDELS and UKIDSS data.
Ref:	=2018MNRAS.475.4148G
by	GALAMETZ A. , PENTERICCI L., CASTELLANO M., MENDEL T., HARTLEY W.G., FOSSATI M., FINOGUENOV A., ALMAINI O., BEIFIORI A., FONTANA A., GRAZIAN A., SCODEGGIO M., KOCEVSKI D.D.
	Mon. Not. R. Astron. Soc., 475, 4148-4169 (2018)
	Growing up in a megalopolis: environmental effects on galaxy evolution in a supercluster at z ~ 0.65 in UKIDSS UDS.
o	Fig. 2, Table 1: <[GPC2018] CN> (Nos C1-C9), <[GPC2018] UNN> (Nos U1-U25), <[GPC2018] U1N> N=1. Table 2: <[GPC2018] UKIDSSNNNNNN> N=379 among (Nos UKIDSS20003-UKIDSS125485).
=E=	Catalogue in electronic form as <J/MNRAS/475/4148/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPC94]
[GPC94]	(Glazebrook+Peacock+Collins+, 1994)
Write:	<<[GPC94] NNNN>>
N:	454
Object:	G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 4: N=287 G + 167 *, among (Nos 22-1661). See also 1995MNRAS.275..169G
Ref:	=1994MNRAS.266...65G
by	GLAZEBROOK K. , PEACOCK J.A., COLLINS C.A., MILLER L.
	Mon. Not. R. Astron. Soc., 266, 65-91 (1994)
	An imaging K-band survey - I. The catalogue, star and galaxy counts.
o	Table 4: <[GPC94] NNNN> N=454 among (Nos 22-1661)
=E=	Catalogue in electronic form as II/211
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPD2009]
[GPD2009]	(Guimaraes+Petitjean+De Carvalho+, 2009) (Not yet in Simbad)
Write:	<<[GPD2009] PSS JHHMM+DDMM abs N.NNN>> <<[GPD2009] SDSS JHHMM+DDMM abs N.NNN>> <<[GPD2009] BRI HHMM+DDMM abs N.NNN>> <<[GPD2009] JHHMM+DDMM abs N.NNN>> <<[GPD2009] PSSHHMM+DDMM abs N.NNN>> (not recognised by Simbad, but found in literature) <<[GPD2009] SDSSHHMM+DDMM abs N.NNN>> <<[GPD2009] BRIHHMM+DDMM abs N.NNN>>
N:	100
Object:	DLA
Note:	Keck ESI spectroscopy of N=100 damped and sub-damped Lyman-α absorber systems.
Ref:	=2009A&A...508..133G
by	GUIMARAES R. , PETITJEAN P., DE CARVALHO R.R., DJORGOVSKI S.G., NOTERDAEME P., CASTRO S., POPPE P.C.R., AGHAEE A.
	Astron. Astrophys., 508, 133-140 (2009)
	Damped and sub-damped Lyman-α absorbers in z > 4 QSOs.
o	Table 2: <[GPD2009] PSS JHHMM+DDMM abs N.NNN>, <[GPD2009] SDSS JHHMM+DDMM abs N.NNN>, <[GPD2009] BRI HHMM+DDMM abs N.NNN>,<[GPD2009] JHHMM+DDMM abs N.NNN>, N=100
=E=	Catalogue in electronic form as <J/A+A/508/133/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPD2011]
[GPD2011]	(Garcia-Benito+Perez+Diaz+, 2011) (Not yet in Simbad)
Write:	<<[GPD2011] NNN>>
Object:	* (SIMBAD class: Star)
Note:	TNG 3.58m telescope ARNICA (NIR) photometry of N=614 stars in NGC 5471. Use of GALEX Nearby Galaxies Survey data and archival HST WFPC2 images.
in source:	NGC 5471
Ref:	=2011AJ....141..126G
by	GARCIA-BENITO R. , PEREZ E., DIAZ A.I., MAIZ-APELLANIZ J., CERVINO M.
	Astron. J., 141, 126 (2011)
	The 100 myr star formation history of NGC 5471 from cluster and resolved stellar photometry.
o	Table 3: <[GPD2011] NNN> (Nos 1-614).
=E=	Catalogue in electronic form as <J/AJ/141/126/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPD88]
[GPD88]	(Garwood+Perley+Dickey+, 1988)
Write:	<<[GPD88] LLL.lll+B.bbb>>
N:	471
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Ref:	=1988AJ.....96.1655G
by	GARWOOD R.W. , PERLEY R.A., DICKEY J.M., MURRAY M.A.
	Astron. J., 96, 1655-1670 (1988)
	A VLA snapshot continuum survey of the first quadrant of the Galactic Plane at 1.5 GHz.
o	Table 2: <[GPD88] LLL.lll+B.bbb> N=471
=E=	Catalogue in electronic form as J/AJ/96/1655
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPD95]
[GPD95]	(Gonzalez-Delgado+Perez+Diaz+, 1995)
Write:	<<[GPD95] NN>> <<[GPD95] A>>
N:	23+5
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	N=23 HII regions, (Nos 1-23). N=3 giant HII regions (Nos A-C), 'N' is the nucleus, 'D' is a partial ring.
in source:	NGC 7714
Ref:	=1995ApJ...439..604G
by	GONZALEZ-DELGADO R.M. , PEREZ E., DIAZ A.I., GARCIA-VARGAS M.L., TERLEVICH E., VILCHEZ J.M.
	Astrophys. J., 439, 604-622 (1995)
	The starburst galaxy NGC 7714.
o	Table 2, text: <[GPD95] NN> (Nos 1-23), <[GPD95] A> (Nos A-C, N).
Ref:	=2000A&A...360..871O
by	O'HALLORAN B. , METCALFE L., DELANEY M., McBREEN B., LAUREIJS R., LEECH K., WATSON D., HANLON L.
	Astron. Astrophys., 360, 871-877 (2000)
	ISO observations of the Wolf-Rayet galaxy NGC 7714 and its companion NGC 7715.
o	Figs 1, 2: <[OMD2000] IR N> (Nos 1-2), <[GPD95] A> (No. D) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPE2000]
[GPE2000]	(Genzel+Pichon+Eckart+, 2000)
Write:	<<[GPE2000] NN.NNA>>
N:	299
Object:	* (SIMBAD class: Star)
Note:	NTT observations. PM* in the central parsec of the Galactic Center. In the format 'NN.NN' stands for the radius or projected separation between the star and Sgr A*. If several stars have the same radius, the second, third, are designated as 'NN.NNB', NN.NNC'.. See also [FGK2003].
in source:	NAME Gal Center
Ref:	=2000MNRAS.317..348G
by	GENZEL R. , PICHON C., ECKART A., GERHARD O.E., OTT T.
	Mon. Not. R. Astron. Soc., 317, 348-374 (2000)
	Stellar dynamics in the Galactic Centre: proper motions and anisotropy.
o	Table 1, col(19): w217 ?? ID not identified (= [GPE2000] 1.34)
o	Table 1, col(1): <[GPE2000] NN.NNA> N=299. Table 1, col(19): <GCIRS NWWN> N=6 added. Table 1, col(19): <[EG97] SNN> (Nos S18-S19) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPE2003]
[GPE2003]	(Greiner+Peimbert+Esteban+, 2003)
Write:	<<[GPE2003] GRB 030329 abs N.NNNN>>
N:	1
Object:	Absorber
Note:	VLT UVES observations. Absorption lines identified in the spectra of GRB 030329.
Ref:	=2003GCN..2020....1G
by	GREINER J. , PEIMBERT M., ESTABAN C., KAUFER A., JAUNSEN A., SMOKE J., KLOSE S., REIMER O.
	GRB Coordinates Network, Circular Service, 2020, 1-None (2003)
	Redshift of GRB 030329.
o	<[GPE2003] GRB 030329 abs N.NNNN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GPEC
GPEC	(Type G, Peculiar)
*****	Avoid the usage of GPEC, prefer [S84]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [GPF2008]
[GPF2008]	(Giardino+Pillitteri+Favata+, 2008)
Write:	<<[GPF2008] Chandra NNN>> <<[GPF2008] XMM NNN>>
N:	262+145
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra and XMM observations of NGC 752.
in source:	NGC 752
Ref:	=2008A&A...490..113G
by	GIARDINO G. , PILLITTERI I., FAVATA F., MICELA G.
	Astron. Astrophys., 490, 113-123 (2008)
	The X-ray luminosity of solar-mass stars in the intermediate age open cluster NGC 752.
o	Table 6: <[GPF2008] Chandra NNN> (Nos 1-262). Table 7: <[GPF2008] XMM NNN> (Nos 1-145).
=E=	Catalogue in electronic form as J/A+A/490/113
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPF97]
[GPF97]	(Graham+Phelps+Freedman+, 1997)
Write:	<<[GPF97] N-N>> <<[GPF97] cNN>>
N:	25+49
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations. Table 3: bright stars in 4 chips (Nos 1-4), format 'N-N'. Chip 1: N=7, Chip 2: N=6, Chip 3: N=6, Chip 4: N=6. Table 25: cepheids in NGC 3351, (Nos c1-c49). Figs 3-5: Finding charts. See also: [FHM94], [HST94], [KIF96], [FFH96], [SHM96], [RMM97], [FBK98], [HHH98], [PSF98], [TFS98], [GHS99], [KIS99], [SHF99], [GFF99], [MHS99], [SFK99], [PKB99], [GSF2000], [MHS2000]
in source:	NGC 3351
Ref:	=1997ApJ...477..535G
by	GRAHAM J.A. , PHELPS R.L., FREEDMAN W.L., SAHA A., FERRARESE L., STETSON P.B., MADORE B.F., SILBERMANN N.A., SAKAI S., KENNICUTT R.C., HARDING P., BRESOLIN F., TURNER A., MOULD J.R., RAWSON D.M., FORD H.C., HOESSEL J.G., HAN M., HUCHRA J.P., MACRI L.M., HUGHES S.M., ILLINGWORTH G.D., KELSON D.D.
	Astrophys. J., 477, 535-559 (1997)
	The Hubble Space Telescope extragalactic distance scale key project. VII. The discovery of cepheids in the Leo I group galaxy NGC 3351.
o	Table 3: <[GPF97] 1-N> N=7, <[GPF97] 2-N> N=6, <[GPF97] 3-N> N=6, <[GPF97] 4-N> N=6. Table 25: <[GPF97] cNN> (Nos c1-c49)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPF98]
[GPF98]	(Giampapa+Prosser+Fleming, 1998)
Write:	<<[GPF98] RNNA>>
N:	15+62
Object:	(X) + * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 11: N=15 X-ray sources in IC 4665, (Nos R1-R15). Table 12: N=62 stars, possible counterparts to the 15 X-ray sources. Finding charts.
in source:	IC 4665
Ref:	=1998ApJ...501..624G
by	GIAMPAPA M.S. , PROSSER C.F., FLEMING T.A.
	Astrophys. J., 501, 624-642 (1998)
	X-ray activity in the open cluster IC 4665.
o	Stars KNN = IC 4665 NN, PNNN = Cl* IC 4665 P NNN.
o	Table 11: <[GPF98] RNN> (Nos R1-R15). Table 12: <[GPF98] RNNA> N=62.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GPFW
GPFW	(Goetz+Pipher+Forrest+Watson+)
Write:	<<GPFW Na>>
N:	3+1
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	WIRO 2.34m telescope NIR observations of point like objects in the region Cep A East.
in source:	Cep A:Cep A East = Cep A East
Ref:	=1998ApJ...504..359G
by	GOETZ J.A. , PIPHER J.L., FORREST W.J., WATSON D.M., RAINES S.N., WOODWARD C.E., GREENHOUSE M.A., SMITH H.A., HUGHES V.A., FISCHER J.
	Astrophys. J., 504, 359-374 (1998)
	Cepheus A East: unraveling the mysteries.
o	Table 3: <GPFW N> (Nos 1-3), <GPFW Na> (No. 1a).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GPG2007]
[GPG2007]	(Goad+Page+Godet+, 2007)
Write:	<<[GPG2007] JHHMMSS.s+DDMMSS.s>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Swift, XRT and UVOT observations of GRB 051117A. An uncatalogued source and a bright stellar source are observed with the XRT.
Ref:	=2007A&A...468..103G
by	GOAD M.R. , PAGE K.L., GODET O., BEARDMORE A., OSBORNE J.P., O'BRIEN P.T., STARLING R., HOLLAND S., BAND D., FALCONE A., GEHRELS N., BURROWS D.N., NOUSEK J.A., ROMING P.W.A., MORETTI A., PERRI M.
	Astron. Astrophys., 468, 103-112 (2007)
	Swift multi-wavelength observations of the bright flaring burst GRB 051117A.
o	Text: <[GPG2007] JHHMMSS.s+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPG2008]
[GPG2008]	(Garcia-Varela+Pietrzynski+Gieren+, 2008)
Write:	<<[GPG2008] cepNN>>
N:	23
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Stat:	is completely incorporated in Simbad
Note:	LCO 1.3m Warsaw telescope, ESO/MPG 2.2m telescope, and CTIO 4m Blanco telescope observations of NGC 247.
in source:	NGC 247
Ref:	=2008AJ....136.1770G
by	GARCIA-VARELA A. , PIETRZYNSKI G., GIEREN W., UDALSKI A., SOSZYNSKI I., WALKER A., BRESOLIN F., KUDRITZKI R.-P., SZEWCZYK O., SZYMANSKI M., KUBIAK M., WYRZYKOWSKI L.
	Astron. J., 136, 1770-1777 (2008)
	The Araucaria project: the distance to the Sculptor group galaxy NGC 247 from cepheid variables discovered in a wide-field imaging survey.
o	Table 5: <[GPG2008] cepNN> (Nos cep01 to cep23).
=E=	Catalogue in electronic form as <J/AJ/136/1770/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPG2012]
[GPG2012]	(Gosnell+Pooley+Geller+, 2012)
Write:	<<[GPG2012] XNN>>
N:	12
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM Newton observations of N=12 X-ray sources within NGC 6819 cluster half-light radius.
in source:	NGC 6819
Ref:	=2012ApJ...745...57G
by	GOSNELL N.M. , POOLEY D., GELLER A.M., KALIRAI J., MATHIEU R.D., FRINCHABOY P., RAMIREZ-RUIZ E.
	Astrophys. J., 745, 57 (2012)
	An unexpected discovery in the rich open cluster NGC 6819 using XMM-Newton.
o	Table 1: <[GPG2012] XNN> (Nos X1-X12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPH2001]
[GPH2001]	(Grady+Polomski+Henning+, 2001)
Write:	<<[GPH2001] JHHMMSS.ss+DDMMSS.s>>
N:	4
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=4 stars close to HD 100546.
Ref:	=2001AJ....122.3396G
by	GRADY C.A. , POLOMSKI E.F., HENNING T., STECKLUM B., WOODGATE B.E., TELESCO C.M., PINA R.K., GULL T.R., BOGGESS A., BOWERS C.W., BRUHWEILER F.C., CLAMPIN M., DANKS A.C., GREEN R.F., HEAP S.R., HUTCHINGS J.B., JENKINS E.B., JOSEPH C., KAISER M.E., KIMBLE R.A., KRAEMER S., LINDLER D., LINSKY J.L., MARAN S.P., MOOS H.W., PLAIT P., ROESLER F., TIMOTHY J.G., WEISTROP D.
	Astron. J., 122, 3396-3406 (2001)
	The disk and environment of the Herbig Be star HD 100546.
o	In abstract D 292.6-7.9 misprint for 296.2 (DCld 296.2-07.9).
o	Table 5: <[GPH2001] JHHMMSS.ss+DDMMSS.s> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPH2009]
[GPH2009]	(Georgiev+Puzia+Hilker+, 2009)
Write:	<<[GPH2009] ENNN-NN-NN>> <<[GPH2009] ICNNNN-NN>> <<[GPH2009] NNNNN-NN>> <<[GPH2009] UNNNN-NN>> <<[GPH2009] DNNN-NN-NN>> <<[GPH2009] DDONN-NN>> <<[GPH2009] KKNNN-NN>> <<[GPH2009] KKHNN-NN>> <<[GPH2009] KKSNN-NN>> <<[GPH2009] UANN-NN>> <<[GPH2009] IKN-NN>>
N:	175
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	Search for globular clusters in 68 nearby dwarf galaxies based on archival HST/ACS images. See also [GGP2008].
Ref:	=2009MNRAS.392..879G
by	GEORGIEV I.Y. , PUZIA T.H., HILKER M., GOUDFROOIJ P.
	Mon. Not. R. Astron. Soc., 392, 879-893 (2009)
	Globular cluster systems in nearby dwarf galaxies - I. HST/ACS observations and dynamical properties of globular clusters at low environmental density.
o	(Erratum) Erratum vol.409 p. 447 (2010)
o	Table 3: <[GPH2009] ENNN-NN-NN>, <[GPH2009] ICNNNN-NN>, <[GPH2009] NNNNN-NN>, <[GPH2009] UNNNN-NN>, <[GPH2009] DNNN-NN-NN>, <[GPH2009] DDONN-NN>, <[GPH2009] KKNNN-NN>, <[GPH2009] KKHNN-NN>, <[GPH2009] KKSNN-NN>, <[GPH2009] UANN-NN>, <[GPH2009] IKN-NN> N=175.
=E=	Catalogue in electronic form as J/MNRAS/392/879
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPH2010]
[GPH2010]	(Galianni+Patat+Higdon+, 2010)
Write:	<<[GPH2010] knot A>> <<[GPH2010] NN>>
N:	2+11
Object:	* + G + Condensation (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	VLT UT2 and FORS2 osbervations of N=2 large stellar condensations (knots A and B) and other sources in the dog-leg tidal stream associated with NGC 1907.
in source:	NGC 1097
Ref:	=2010A&A...521A..20G
by	GALIANNI P. , PATAT F., HIGDON J.L., MIESKE S., KROUPA P.
	Astron. Astrophys., 521A, 20-20 (2010)
	VLT observations of NGC 1097's ``dog-leg'' tidal stream. Dwarf spheroidals and tidal streams.
o	Fig. 1, Table 1: <[GPH2010] knot A> (Nos A-B), <[GPH2010] NN> (Nos 1-11).
o	Paragraph 4. Mayal I is a probable misprint for Mayall II.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPI2003]
[GPI2003]	(Guseva+Papaderos+Izotov+, 2003) (Not yet in Simbad)
Write:	<<[GPI2003] aN>> <<[GPI2003] eN>>
N:	4+4
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Note:	HST image and Continuum-substracted H-alpha image of SBSG 1415+437. (Nos a1-a4) are regions with hydrogen absorption lines. (Nos e1-e4) are regions with hydrogen emission lines.
in source:	SBSG 1415+437
Ref:	=2003A&A...407..105G
by	GUSEVA N.G. , PAPADEROS P., IZOTOV Y.I., GREEN R.F., FRICKE K.J., THUAN T.X., NOESKE K.G.
	Astron. Astrophys., 407, 105-120 (2003)
	Spectroscopic and photometric studies of low-metallicity star-forming dwarf galaxies. III. SBS 1415+437.
o	Table 6 : designations 'NN' in column 1 not in Simbad, CG 1116+51 = ACG 1116+51, I Zw 18C = [VWH98] HI-C.
o	Figs 1, 2, Table 3: <[GPI2003] aN> (Nos a1-a4, e1-e4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GPIPS
GPIPS	(Galactic Plane Infrared Polarization Survey)
Write:	<<GPIPS JHHMMSS.ss+DDMMSS.s>>
N:	13861329
Object:	* (SIMBAD class: Star)
Note:	1.8m Perkins telescope Mimir NIR observations of N=13861329 stars in the northern Galactic plane.
Ref:	=2012ApJS..200...21C
by	CLEMENS D.P. , PAVEL M.D., CASHMAN L.R.
	Astrophys. J., Suppl. Ser., 200, 21 (2012)
	The Galactic Plane Infrared Polarization Survey (GPIPS): data release 1.
o	<GPIPS JHHMMSS.ss+DDMMSS.s> N=?
Ref:	=2020ApJS..249...23C
by	CLEMENS D.P. , CASHMAN L.R., CERNY C., EL-BATAL A.M., JAMESON K.E., MARCHWINSKI R., MONTGOMERY J., PAVEL M., PINNICK A., TAYLOR B.W.
	Astrophys. J., Suppl. Ser., 249, 23-23 (2020)
	The Galactic Plane Infrared Polarization Survey (GPIPS): Data Release 4.
o	<GPIPS JHHMMSS.ss+DDMMSS.s> N=13861329.
=E=	Catalogue in electronic form as <J/ApJS/249/23/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GPJ2005]
[GPJ2005]	(Guainazzi+Piconcelli+Jimenez-Bailon+, 2005)
Write:	<<[GPJ2005] W>>
N:	2
Object:	G in Pair (SIMBAD class: GinPair = Galaxy in Pair of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of the galaxy pair ESO 509-66. The pair id composed of two obscured AGN observed as X-ray sources.
in source:	ESO 509-66
Ref:	=2005A&A...429L...9G
by	GUAINAZZI M. , PICONCELLI E., JIMENEZ-BAILON E., MATT G.
	Astron. Astrophys., 429, 9-12 (2005)
	The early stage of a cosmic collision? XMM-Newton unveils two obscured AGN in the galaxy pair ESO509-IG066.
o	MGC 2214+3350 is amisprint for MITG J2214+3550.
o	Table 1: <[GPJ2005] W> (Nos W, E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPJ2008]
[GPJ2008]	(Gurney+Plume+Johnstone, 2008)
Write:	<<[GPJ2008] Source N>>
N:	9
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	JCMT SCUBA and Spitzer IRAC and MIPS observations of the Oph Molecular Cloud.
in source:	NAME rho Oph Cloud
Ref:	=2008PASP..120.1193G
by	GURNEY M. , PLUME R., JOHNSTONE D.
	PASP, 120, 1193-1206 (2008)
	Molecular tracers of embedded star formation in Ophiuchus.
o	Table 1: <[GPJ2008] Source N> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GPK
GPK	(Gonzalez-Perez+Kidger+)
*****	Avoid the usage of GPK, prefer [GKM2001]
Origin	of the Acronym: L (2005MNRAS.356..336O)
Details on Acronym: [GPK2020]
[GPK2020]	(Goicoechea+Pabst+Kabanovic+, 2020)
Write:	<<[GPK2020] NN>>
N:	10
Object:	CO Globule (SIMBAD class: Globule = Globule (low-mass dark cloud))
Stat:	is completely incorporated in Simbad
Note:	IRAM 30m telescope 12CO, 13CO, and C18O (J = 2-1) observations of N=10 CO globules in Orion's Veil.
in source:	NAME Orion's Veil
Ref:	=2020A&A...639A...1G
by	GOICOECHEA J.R. , PABST C.H.M., KABANOVIC S., SANTA-MARIA M.G., MARCELINO N., TIELENS A.G.G.M., HACAR A., BERNE O., BUCHBENDER C., CUADRADO S., HIGGINS R., KRAMER C., STUTZKI J., SURI S., TEYSSIER D., WOLFIRE M.
	Astron. Astrophys., 639A, 1-1 (2020)
	Molecular globules in the Veil bubble of Orion. IRAM 30 m ^{12}CO, ^{13}CO, and C^{18}O (2-1) expanded maps of Orion A.
o	Fig. 3, Table 1: <[GPK2020] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GPM
GPM	(General catalog of Proper Motions stars)
Write:	<<GPM DDD.dddddd+DD.dddddd>>
N:	52805
Object:	* (SIMBAD class: Star)
Note:	New version of the general compiled catalogue of absolute proper motions.
Ref:	=1997KFNT...13e..70R
by	RYBKA S.P. , YATSENKO A.I.
	Kinematika Fiz. Nebesn. Tel., 13, part no 5, 70-74 (1997)
	GPM - compiled catalogue of absolute proper motions of stars in selected areas of sky with galaxies.
o	<GPM DDD.dddddd-DD.dddddd> N=52805.
=E=	Catalogue in electronic form as I/285
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GPM1
GPM1	(General catalog of Proper Motions stars, 1st version)
Write:	<<GPM1 NNN>>
N:	977
Object:	* (SIMBAD class: Star)
Note:	General compiled catalogue of absolute proper motion for a sample of Hipparcos stars (HIP).
Ref:	=1997A&AS..121..243R
by	RYBKA S.P. , YATSENKO A.I.
	Astron. Astrophys., Suppl. Ser., 121, 243-246 (1997)
	GPM1 - a catalog of absolute proper motions of stars with respect to galaxies.
o	Table 2: <GPM1 NNN> (Nos 1-977)
=E=	Catalogue in electronic form as J/A+AS/121/243
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GPM2004]
[GPM2004]	(Gomez+Persi+Marenzi+, 2004)
Write:	<<[GPM2004] AN>>
N:	4+5
Object:	H2 Knot (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	ESO NTT near-IR observations of the Chameleon I cloud. Seven H2 emission knots are found in the northern area of the cloud.
in source:	NAME Cha I
Ref:	=2004A&A...423..629G
by	GOMEZ M. , PERSI P., MARENZI A.R., ROTH M., TAPIA M.
	Astron. Astrophys., 423, 629-641 (2004)
	A search for shock-excited molecular hydrogen knots in Chamaeleon I very low mass YSOs.
o	Table 2: <[GPM2004] AN> (Nos A-D, B1-B2, C1-C3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPM2009]
[GPM2009]	(Guseva+Papaderos+Meyer+, 2009)
Write:	<<[GPM2009] JHHMM+DDMM N>> <<[GPM2009] JHHMM+DDMM BGN>> <<[GPM2009] NNNNNN>> <<[GPM2009] GHHMMSSs+DDMMSS N>> <<[GPM2009] GHHMMSSs+DDMMSS BG>> <<[GPM2009] HHMM+DDMM>> <<[GPM2009] PHL293B>>
N:	38+28
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 and ESO 3.6m telescope EFOSC2 spectroscopy of HII regions in emission-line galaxies.
Ref:	=2009A&A...505...63G
by	GUSEVA N.G. , PAPADEROS P., MEYER H.T., IZOTOV Y.I., FRICKE K.J.
	Astron. Astrophys., 505, 63-72 (2009)
	An investigation of the luminosity-metallicity relation for a large sample of low-metallicity emission-line galaxies.
o	Tables 1, 2: <[GPM2009] JHHMM+DDMM N>, <[GPM2009] JHHMM+DDMM {BG}N>, <[GPM2009] NNNNNN>, <[GPM2009] GHHMMSSs+DDMMSS N>, <[GPM2009] GHHMMSSs+DDMMSS {BG}>, <[GPM2009] HHMM+DDMM>, <[GPM2009] PHL293B> N=38+28.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPM2011]
[GPM2011]	(Graur+Poznanski+Maoz+, 2011)= (SNSDF) = (hSDF)
Write:	<<[GPM2011] SNSDF YYMM.NN>> <<[GPM2011] hSDF YYMM.NN>>
N:	190+190
Object:	SN + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Subaru telescope observations of the SDF to search for supernovae and their host galaxies. Keck LRIS and DEIMOS spectroscopy. See SNSDF and hSDF.
in source:	NAME SDF
Ref:	=2011MNRAS.417..916G
by	GRAUR O. , POZNANSKI D., MAOZ D., YASUDA N., TOTANI T., FUKUGITA M., FILIPPENKO A.V., FOLEY R.J., SILVERMAN J.M., GAL-YAM A., HORESH A., JANNUZI B.T.
	Mon. Not. R. Astron. Soc., 417, 916-940 (2011)
	Supernovae in the Subaru Deep Field: the rate and delay-time distribution of type Ia supernovae out to redshift 2.
o	The SNSDF names in this reference are not the same than in 2007MNRAS.382.1169P. That's why the CDS team had to create an acronym [GPM2011].
o	Table 2: <[GPM2011] SNSDF YYMM.NN> N=190. Table 3: <[GPM2011] hSDF YYMM.NN> N=190.
=E=	Catalogue in electronic form as J/MNRAS/417/916
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GPN
GPN	(Galactic Planetary Nebula) (Not yet in Simbad)
**	catalog: use PN
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GPO2007]
[GPO2007]	(Godet+Page+Osborne+, 2007)
Write:	<<[GPO2007] JHHMMSS.ss+DDMMSS.s>> <<[GPO2007] SX>>
N:	1+1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Swift BAT and XRT observations of X-ray sources in the field of GRB 050822.
Ref:	=2007A&A...471..385G
by	GODET O. , PAGE K.L., OSBORNE J., ZHANG B., BURROWS D.N., O'BRIEN P.T., HILL J.E., RACUSIN J., BEARDMORE A.P., GOAD M.R., FALCONE A., MORRIS D.C., ZIAEEPOUR H.
	Astron. Astrophys., 471, 385-394 (2007)
	GRB050822: detailed analysis of an XRF observed by Swift.
o	Paragraph 4.3.3 GRB 050202B is a misprint for GRB 050502B.
o	Paragr.2.1: <[GPO2007] JHHMMSS.ss+DDMMSS.s> N=1, Paragr.3.1: <[GPO2007] SX> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GPPS
GPPS	(Galactic Plane Pulsar Snapshot)
Write:	<<GPPS NNNN>>
Object:	Psr (SIMBAD class: Pulsar)
Note:	The FAST Galactic Plane Pulsar Snapshot survey list of pulsars. More information, including the updated list of discovered pulsars, available at: http://zmtt.bao.ac.cn/GPPS/ Only the first reference listing GPPS sources is given here.
Ref:	=2021RAA....21..107H
by	HAN J.L. , WANG C., WANG P.F., WANG T., ZHOU D.J., SUN J.-H., YAN Y., SU W.-Q., JING W.-C., CHEN X., GAO X.Y., HOU L.-G., XU J., LEE K.J., WANG N., JIANG P., XU R.-X., YAN J., GAN H.-Q., GUAN X., HUANG W.-J., JIANG J.-C., LI H., MEN Y.-P., SUN C., WANG B.-J., WANG H.G., WANG S.-Q., XIE J.-T., XU H., YAO R., YOU X.-P., YU D.J., YUAN J.-P., YUEN R., ZHANG C.-F., ZHU Y.
	RAA, 21, 107-107 (2021)
	The FAST Galactic Plane Pulsar Snapshot survey: I. Project design and pulsar discoveries.
o	Table 2: <GPPS NNNN> (Nos 1-201).
=E=	Catalogue in electronic form as <J/other/RAA/21.107/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GPR2013]
[GPR2013]	(Gaczkowski+Preibisch+Ratzka+, 2013)
Write:	<<[GPR2013] JHHMMSS.s+DDMMSS>>
N:	1142
Object:	(FIR) (SIMBAD class: FarIR = Far-IR source (λ >= 30 µm))
Note:	Herschel PACS and SPIRE observations of the Carina Nebula Complex.
in source:	NAME Carina Nebula
Ref:	=2013A&A...549A..67G
by	GACZKOWSKI B. , PREIBISCH T., RATZKA T., ROCCATAGLIATA V., OHLENDORF H., ZINNECKER H.
	Astron. Astrophys., 549A, 67-67 (2013)
	Herschel far-infrared observations of the Carina Nebula complex. II. The embedded young stellar and protostellar population.
o	Tables A.1, B.1, C.1, D.1: <[GPR2013] JHHMMSS.s+DDMMSS> N=1142.
=E=	Catalogue in electronic form as J/A+A/549/A67
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GPS
GPS	(Gigahertz Peaked Spectrum)
*****	Avoid the usage of GPS, prefer Gopal
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GPS
GPS	(Gal. Plane Survey)
Write:	<<GPS HHMM+DDd>>
N:	70
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Distribution of 2-6 keV X-ray emission in the galactic plane in the first and fourth galactic quadrants, a series of scanning observations with the medium-energy proportional counters on EXOSAT.
Ref:	=1988MNRAS.232..551W
by	WARWICK R.S. , NORTON A.J., TURNER M.J.L., WATSON M.G., WILLINGALE R.
	Mon. Not. R. Astron. Soc., 232, 551-564 (1988)
	A survey of the galactic plane with EXOSAT.
o	Table 2: <GPS HHMM+DDd>, N=70
Details on Acronym: GPS
GPS	(Gal. Plane Survey)
*****	Avoid the usage of GPS, prefer GPSR
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GPS
GPS	(Gal. Plane Survey)
*****	Avoid the usage of GPS, prefer GPSR5
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GPS2005]
[GPS2005]	(Gorosabel+Perez-Ramirez+Sollerman+, 2005)
Write:	<<[GPS2005] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS observations of a galaxy near the host galaxy of GRB 030329.
Ref:	=2005A&A...444..711G
by	GOROSABEL J. , PEREZ-RAMIREZ D., SOLLERMAN J., DE UGARTE POSTIGO A., FYNBO J.P.U., CASTRO-TIRADO A.J., JAKOBSSON P., CHRISTENSEN L., HJORTH J., JOHANNESSON G., GUZIY S., CASTRO CERON J.M., BJOERNSSON G., SOKOLOV V.V., FATKHULLIN T.A., NILSSON K.
	Astron. Astrophys., 444, 711-721 (2005)
	The GRB 030329 host: a blue low metallicity subluminous galaxy with intense star formation.
o	The host galaxy of GRB 030329 = [GPE2003] GRB 030329 abs 0.1685
o	Paragr. 3.6: <[GPS2005] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPS2008]
[GPS2008]	(Greve+Pope+Scott+, 2008)= (GN) = (MM)
Write:	<<[GPS2008] MM JHHMMSS+DDMMSS>> <<[GPS2008] GN 1200.NN>>
N:	47
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	IRAM 30m MAMBO 1200mu.m observations of the GOODS North Field.
in source:	NAME GOODS North Field
Ref:	=2008MNRAS.389.1489G
by	GREVE T.R. , POPE A., SCOTT D., IVISON R.J., BORYS C., CONSELICE C.J., BERTOLDI F.
	Mon. Not. R. Astron. Soc., 389, 1489-1506 (2008)
	A 1200-µm MAMBO survey of the GOODS-N field: a significant population of submillimetre dropout galaxies.
o	Table 1: <[GPS2008] MM JHHMMSS+DDMMSS> N=47 = <[GPS2008] GN 1200.NN> (Nos 1-47).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPS2012]
[GPS2012]	(Gusev+Pilyugin+Sakhibov+, 2012)
Write:	<<[GPS2012] NGC NNNN NN>>
N:	63
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	SAO 6m telescope SCORPIO spectroscopic observations of N=63 HII regions in six spiral galaxies (NGC 628, NGC 783, NGC 2336, NGC 6217, NGC 7331 and NGC 7678).
in source:	NGC 628
in source:	NGC 783
in source:	NGC 2336
in source:	NGC 6217
in source:	NGC 7331
in source:	NGC 7678
Ref:	=2012MNRAS.424.1930G
by	GUSEV A.S. , PILYUGIN L.S., SAKHIBOV F., DODONOV S.N., EZHKOVA O.V., KHRAMTSOVA M.S.
	Mon. Not. R. Astron. Soc., 424, 1930-1940 (2012)
	Oxygen and nitrogen abundances of HII regions in six spiral galaxies.
o	Tables 3-5: <[GPS2012] NGC NNNN NN> N=63.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPS2015]
[GPS2015]	(Gaczkowski+Preibisch+Stanke+, 2015)
Write:	<<[GPS2015] NN>>
N:	15
Object:	Core (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	APEX LABOCA 870µm continuum observations of N=15 cores in the Lupus I molecular cloud. Use of archival Herschel and Planck data.
in source:	NAME Lupus I = Lupus 1
Ref:	=2015A&A...584A..36G
by	GACZKOWSKI B. , PREIBISCH T., STANKE T., KRAUSE M.G.H., BURKERT A., DIEHL R., FIERLINGER K., KROELL D., NGOUMOU J., ROCCATAGLIATA V.
	Astron. Astrophys., 584A, 36-36 (2015)
	Squeezed between shells? The origin of the Lupus I molecular cloud. APEX/LABOCA, Herschel, and Planck observations.
o	Table 3: <[GPS2015] NN> (Nos 1-15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GPSA
GPSA	(GLIMPSE Point Source Archive)
*****	Avoid the usage of GPSA, prefer SSTGLMA
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GPSC
GPSC	(GLIMPSE Point Source Catalog)
*****	Avoid the usage of GPSC, prefer SSTGLMC
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GPSR
GPSR	(Gal. Plane Survey, Radio-source)= (GPS) = (GPSR1.4) = (ZGS)
Write:	<<GPSR LLL.lll+B.bbb>>
N:	3454
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ref. 1994ApJS...91..347B, table 2: 5 new sources GPSR (1.4GHz), marked with an N.
Ref:	=1990ApJS...74..181Z
by	ZOONEMATKERMANI S. , HELFAND D.J., BECKER R.H., WHITE R.L., PERLEY R.A.
	Astrophys. J., Suppl. Ser., 74, 181-224 (1990)
	A catalog of small-diameter radio sources in the galactic plane.
o	Table 4: <GPSR LLL.lll+BB.bbb> N=1992
Ref:	=1992ApJS...80..211H
by	HELFAND D.J. , ZOONEMATKERMANI S., BECKER R.H., WHITE R.L.
	Astrophys. J., Suppl. Ser., 80, 211-255 (1992)
	Compact radio sources near the galactic plane.
o	Table 3: <GPSR LLL.lll+BB.bbb> N=1457
Ref:	=1994ApJS...91..347B
by	BECKER R.H. , WHITE R.L., HELFAND D.J., ZOONEMATKERMANI S.
	Astrophys. J., Suppl. Ser., 91, 347-387 (1994)
	A 5GHz VLA survey of the galactic plane.
o	Table 2: <GPSR5 LLL.lll+B.bbb> N=1272, <GPSR LLL.lll+B.bbb> N=5
=E=	Catalogue in electronic form as J/ApJS/74/181
=E=	Catalogue in electronic form as <J/ApJS/80/211/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: GPSR1.4
GPSR1.4	(Gal. Plane Survey, Radio-source, 1.4 GHz)
*****	Avoid the usage of GPSR1.4, prefer GPSR
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GPSR5
GPSR5	(Gal. Plane Survey, Radio-source, 5 GHz)= (GPS)
Write:	<<GPSR5 LLL.lll+B.bbb>>
N:	1272
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1994ApJS...91..347B
by	BECKER R.H. , WHITE R.L., HELFAND D.J., ZOONEMATKERMANI S.
	Astrophys. J., Suppl. Ser., 91, 347-387 (1994)
	A 5GHz VLA survey of the galactic plane.
o	Table 2: <GPSR5 LLL.lll+B.bbb> N=1272, <GPSR LLL.lll+B.bbb> N=5
=E=	Catalogue in electronic form as J/ApJS/91/347
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: GPSV
GPSV	(Galactic Plane Survey Variable) (Not yet in Simbad)
*****	Avoid the usage of GPSV, prefer [CLF2014]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GPT94]
[GPT94]	(Gonzalez-Delgado+Perez+Tenorio-Tagle+. 1994)
Write:	<<[GPT94] Knot A>>
N:	2
Object:	H-alpha Knot (SIMBAD class: PartofCloud = Part of Cloud)
Note:	See also [DRR2000].
in source:	NGC 2363
Ref:	=1994ApJ...437..239G
by	GONZALEZ-DELGADO R.M. , PEREZ E., TENORIO-TAGLE G., VILCHEZ J.M., TERLEVICH E., TERLEVICH R., TELLES E., RODRIGUEZ-ESPINOSA J.M., MAS-HESSE J.M., GARCIA-VARGAS M.L., DIAZ A.I., CEPA J., CASTANEDA H.
	Astrophys. J., 437, 239-261 (1994)
	Violent star formation in NGC 2363.
o	(Erratum) erratum 1996 vol.473 p.1125
o	NGC 2366 I and II = [M94c] NGC 2366 1 and 2.
o	Fig.2: <[GPT94] Knot A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPV2018]
[GPV2018]	(Guglielmo+Poggianti+Vulcani+, 2018) (Not yet in Simbad)
Write:	<<[GPV2018] DDD.dddd+DD.ddddd>>
N:	24336
Object:	G (SIMBAD class: Galaxy)
Note:	Spectrophotometric catalog of N=24336 galaxies taken from the XXL-North region.
Ref:	=2018A&A...620A...7G
by	GUGLIELMO V. , POGGIANTI B.M., VULCANI B., ADAMI C., GASTALDELLO F., ETTORI S., FOTOUPOULOU S., KOULOURIDIS E., RAMOS CEJA M.E., GILES P., McGEE S., ALTIERI B., BALDRY I., BIRKINSHAW M., BOLZONELLA M., BONGIORNO A., BROWN M., CHIAPPETTI L., DRIVER S., ELYIV A., EVRARD A., GARILLI B., GROOTES M., GUENNOU L., HOPKINS A., HORELLOU C., IOVINO A., LIDMAN C., LISKE J., MAUROGORDATO S., OWERS M., PACAUD F., PALTANI S., PIERRE M., PLIONIS M., PONMAN T., ROBOTHAM A., SADIBEKOVA T., SCODEGGIO M., SERENO M., SMOLCIC V., TUFFS R., VALTCHANOV I., VIGNALI C., WILLIS J.
	Astron. Astrophys., 620A, 7-7 (2018)
	The XXL Survey. XXII. The XXL-North spectrophotometric sample and galaxy stellar mass function in X-ray detected groups and clusters.
o	Table IX/52/xxlngal: <[GPV2018] DDD.dddd+DD.ddddd> N=24336.
=E=	Catalogue in electronic form as IX/52/xxlngal
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GPW2005]
[GPW2005]	(Gogus+Patel+Wilson+, 2005)
Write:	<<[GPW2005] NN>>
N:	12
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Optical and infrared counterparts of the transient from the Tubitak National Observatory and 2MASS respectively.
Ref:	=2005ApJ...632.1069G
by	GOGUS E. , PATEL S.K., WILSON C.A., WOODS P.M., FINGER M.H., KOUVELIOTOU C.
	Astrophys. J., 632, 1069-1074 (2005)
	Chandra localization of XTE J1906+090 and discovery of its optical and infrared counterparts.
o	(Erratum) erratum vol. 637, p. 553 (2006)
o	Table 1: <[GPW2005] NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GPX
GPX	(Galactic Plane eXoplanet)
Write:	<<GPX -Na>> <<GPX -TFNNA-NNNN>>
N:	?
Object:	* (SIMBAD class: Star)
Note:	The Galactic plane eXoplanet (GPX) survey performs photometric observations of the Galactic plane to search for new transiting exoplanets.
Ref:	=2020MNRAS.493.5208K
by	KRUSHINSKY V. , BENNI P., BURDANOV A., ANTOKHIN I., ANTOKHINA E., JEHIN E., BARKAOUI K., FITZSIMMONS A., GIBSON C., GILLON M., POPOV A., BASTURK O., BENKHALDOUN Z., MARCHINI A., PAPINI R., SALVAGGIO F., BRAZHKO V.
	Mon. Not. R. Astron. Soc., 493, 5208-5217 (2020)
	Discovery of a pre-cataclysmic binary with unusual chromaticity of the eclipsed white dwarf by the GPX survey.
o	Fig. 1, Table 1: <GPX-TF-NNA-NNNN> (No. -TF16E-48).
Ref:	=2021MNRAS.505.4956B
by	BENNI P. , BURDANOV A.Y., KRUSHINSKY V.V., BONFANTI A., HEBRARD G., ALMENARA J.M., DALAL S., DEMANGEON O.D.S., TSANTAKI M., PEPPER J., STASSUN K.G., VANDERBURG A., BELINSKI A., KASHAEV F., BARKAOUI K., KIM T., KANG W., ANTONYUK K., DYACHENKO V.V., RASTEGAEV D.A., BESKAKOTOV A., MITROFANOVA A.A., POZUELOS F.J., KUZNETSOV E.D., POPOV A., KIEFER F., WILSON P.A., RICKER G., VANDERSPEK R., LATHAM D.W., SEAGER S., JENKINS J.M., SOKOV E., SOKOVA I., MARCHINI A., PAPINI R., SALVAGGIO F., BANFI M., BASTURK O., TORUN S., YALCINKAYA S., IVANOV K., VALYAVIN G., JEHIN E., GILLON M., PAKSTIENE E., HENTUNEN V.-P., SHADICK S., BRETTON M., WUNSCHE A., GARLITZ J., JONGEN Y., MOLINA D., GIRARDIN E., GRAU HORTA F., NAVES R., BENKHALDOUN Z., JONER M.D., SPENCER M., BIERYLA A., STEVENS D.J., JENSEN E.L.N., COLLINS K.A., CHARBONNEAU D., QUINTANA E.V., MULLALLY S.E., HENZE C.E.
	Mon. Not. R. Astron. Soc., 505, 4956-4967 (2021)
	Discovery of a young low-mass brown dwarf transiting a fast-rotating F-type star by the Galactic Plane eXoplanet (GPX) survey.
o	Fig. 1, Table 1: <GPX-Na> (Nos 1, 1b), <GPX-TF-NNA-NNNN> (No. -TF18A-1859).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GQH2007]
[GQH2007]	(Gouliermis+Quanz+Henning, 2007)
Write:	<<[GQH2007] NN>>
N:	22
Object:	Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Note:	Spitzer-IRAC photometry of the star-forming HII region LHA 115-N 90.
in source:	Magellanic Clouds:SMC:LHA 115-N 90 = LHA 115-N 90
Ref:	=2007ApJ...665..306G
by	GOULIERMIS D.A. , QUANZ S.P., HENNING T.
	Astrophys. J., 665, 306-314 (2007)
	Clustered star formation in the Small Magellanic Cloud. A Spitzer/IRAC view of the star-forming region NGC 602/N 90.
o	Table 1: <[GQH2007] NN> N=22 among (Nos 1-57).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Gr
Gr	(Greenwich obs.)
*****	Avoid the usage of Gr, prefer AC
Details on Acronym: Gr
Gr	(Greenstein)
*****	Avoid the usage of Gr, prefer EGGR
Details on Acronym: Gr
Gr	(Groombridge)
*****	Avoid the usage of Gr, prefer Gmb
Details on Acronym: GR
GR	(Giclas, Red *)
*****	Avoid the usage of GR, prefer GR*
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Gr
Gr	(Grakovo Radio obs.)
*****	Avoid the usage of Gr, prefer Gra
Details on Acronym: GR
GR	(G. Reaves)
*****	Avoid the usage of GR, prefer GRDG
Details on Acronym: GR
GR	(Glass+Reid)
*****	Avoid the usage of GR, prefer GRRV
Details on Acronym: GR
GR	(G. Romano)
Write:	<<*SV GR** NNN>>
N:	292
Object:	V* (SIMBAD class: Variable* = Variable Star)
Rem:	V* Nomenclature.
Auth.:	ROMANO G.
Details on Acronym: GR
GR	(Group of G)
*****	Avoid the usage of GR, prefer [V84]
Details on Acronym: GR*
GR*	(Giclas, Red *)= (GR)
Write:	<<GR* NNN>>
N:	504
Object:	Red * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	1980LowOB...8..157G: Recapitulation of the complete catalogue in order of right ascension.
Ref:	=1972LowOB...7..217G
by	GICLAS H.L. , BURNHAM R., THOMAS N.G.
	Lowell Obs. Bull., 7, 217-254 (1972)
	Proper motion survey at the South Galactic Pole. Lists of white dwarf suspects. List of very red stars.
o	Plates 266-269
o	<GR* NN> (Nos 1-47). <GD NNN> (Nos 563-952)
Ref:	=1973LowOB...7..273G
by	GICLAS H.L. , BURNHAM R., THOMAS N.G.
	Lowell Obs. Bull., 7, 273-None (1973)
	Proper motion Survey at the South Galactic Pole . Lists of very red stars,.
o	Plates 270-271
o	<GR* NNN> (Nos 48-119)
Ref:	=1975LowOB...8....9G
by	GICLAS H.L. , BURNHAM R., THOMAS N.G.
	Lowell Obs. Bull., 8, 9-49 (1975)
	Lowell proper motions. XVII.
o	Plates 272-273
o	<GR* NNN> (Nos 120-288). <GD NNNN> (Nos 953-1338).
Ref:	=1978LowOB...8...51G
by	GICLAS H.L. , BURNHAM R., THOMAS N.G.
	Lowell Obs. Bull., 8, 51-88 (1978)
	Lowell proper motions. XVIII.
o	Plates 274-275
o	<GR* NNN> (Nos 289-504). <GD NNNN> (Nos 1339-1712)
=E=	Catalogue in electronic form as <I/316/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 5GR
5GR	(Group of Radio-sources with N>=5)
Write:	<<5GR NNNN.NN>>
N:	35
Object:	Group of Radios (SIMBAD class: Radio = Radio Source)
Note:	Search for groups of radio-sources from the FIRST catalog with no fewer than five sources. See also CGR-F.
Ref:	=2003AstL...29..224G
by	GUBANOV A.G. , KOPYLOV A.I., POTAPOV A.S.
	Astron. Lett., 29, 224-235 (2003)
	Search for groups of extragalactic radio sources.
o	Table: <5GR NNNN.NN> N=35 = <CGR-F JHHMMSS.s+DDMMSS> N=35.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GR92]
[GR92]	(Ghosh+Rao, 1992)
Write:	<<[GR92] HHMM+DDd>>
N:	134
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=96 extragal. sources. Table 2: N=14 control sources. Table 3: N=24 calibration sources
Ref:	=1992A&A...264..203G
by	GHOSH T. , RAO A.P.
	Astron. Astrophys., 264, 203-216 (1992)
	Low-frequency variability and the galactic distribution of electron-density fluctuation.
o	Tables 1, 2, 3: <[GR92] HHMM+DDd> N=96+14+24
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GR99]
[GR99]	(Gomez de Castro+Robles, 1999)= ([GR99a])
Write:	<<[GR99] HHMMSS.ss+DDMMSS.s>> <<[GR99] Knot N>>
N:	1+5
Object:	Knot (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=1 faint VLA source '214214.90+655443.0'. Table 3: N=5 main knots in GGD 34. See also [GME93].
in source:	GGD 34
Ref:	=1999A&A...344..632G
by	GOMEZ DE CASTRO A.I. , ROBLES A.
	Astron. Astrophys., 344, 632-638 (1999)
	The origin of the protostellar jet GGD 34.
o	Table 2: <[GR99] 214214.90+655443.0> N=1. Table 3: <[GR99] Knot N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GR99a]
[GR99a]	(Gomez de Castro+Robles, 1999)
*****	Avoid the usage of [GR99a], prefer [GR99]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GR99b]
[GR99b]	(Gubanov+Reshetnikov, 1999)
Write:	<<[GR99b] ANNNN.NN>>
N:	383
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Identification of radio-sources in 26 rich galactic clusters from the FIRST survey.
Ref:	=1999AstL...25..380G
by	GUBANOV A.G. , RESHETNIKOV V.P.
	Astron. Lett., 25, 380-388 (1999)
	Identification of radio sources in clusters of galaxies.
o	1999PAZh...25..447G
o	Table 2: <[GR99b] ANNNN.NN> N=383.
=E=	Catalogue in electronic form as J/PAZh/25/447
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Gra
Gra	(Grakovo Radio obs.)= (Gr)
Write:	<<Gra HHMM+DDA>> <<Gra JHHMM+DDA>>
N:	1819+483
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	UTR-2 decametric radio telescope observations. Numbering 'NNN' not used.
Ref:	=1978Ap&SS..54...37B
by	BRAUDE S.Y. , MEGN A.V., RASHKOVSKI S.L., RYABOV B.P., SHARYKIN N.K., SOKOLOV K.P., TKATCHENKO A.P., ZHOUK I.N.
	Astrophys. Space Sci., 54, 37-128 (1978)
	Decametric survey of discrete sources in the northern sky. II. Source catalogue in the range of declinations +10 to +20.
o	Table 1: <Gra HHMM+DDA> N=329
Ref:	=1979Ap&SS..64...73B
by	BRAUDE S.Y. , MEGN A.V., SOKOLOV K.P., TKATCHENKO A.P., SHARYKIN N.K.
	Astrophys. Space Sci., 64, 73-126 (1979)
	Decametric survey of discrete sources in the northern sky. V. Source catalogue in the range of declinations 0 to +10.
o	Table I: <Gra HHMM+DDA> N=364
Ref:	=1981Ap&SS..74..409B
by	BRAUDE S.Y. , MIROSHNITCHENKO A.P., SOKOLOV K.P., SHARYKIN N.K.
	Astrophys. Space Sci., 74, 409-451 (1981)
	Decametric survey of discrete sources. VII. Source catalogue in the range of declination -2 to -13.
o	PKS 0420-08 for PKS 0421-090; PKS 0822-09 = MRC 0822-096; PKS 1150-04 for MRC 1150-044
o	Table I: <Gra HHMM+DDA> N=316
Ref:	=1985Ap&SS.111....1B
by	BRAUDE S.Y. , SHARYKIN N.K., SOKOLOV K.P., ZAKCHARENKO S.M.
	Astrophys. Space Sci., 111, 1-64 (1985)
	Decametric survey of discrete sources in the northern sky. IX. Source catalogue in the declination range 52 °. to 60 °.
o	Table II: <Gra HHMM+DDA> N=313
Ref:	=1994Ap&SS.213....1B
by	BRAUDE S.Y. , SOKOLOV K.P., ZAKHARENKO S.M.
	Astrophys. Space Sci., 213, 1-61 (1994)
	Decametric survey of discrete sources in the northern sky. XI. The results of the UTR-2 very low-frequency sky survey in the declination range 41 °. to 52 °.
o	Appendix: <Gra HHMM+DDA> N=432
Ref:	=1995Ap&SS.226..245B
by	BRAUDE S.Y. , SOKOLOV K.P., SHARYKIN N.K., ZAKHARENKO S.M.
	Astrophys. Space Sci., 226, 245-271 (1995)
	Decametric survey of discrete sources in the northern sky. XII. Spectra of some radio sources in the frequency range 12.6 to 1400 MHz for declinations 41° to 52°.
o	<Gra HHMM+DD> N=194
Ref:	=2002Ap&SS.280..235B
by	BRAUDE S.Y. , RASHKOVSKY S.L., SIDORCHUK K.M., SIDORCHUK M.A., SOKOLOV K.P., SHARYKIN N.K., ZAKHARENKO S.M.
	Astrophys. Space Sci., 280, 235-299 (2002)
	Decametric survey of discrete sources in the northern sky. XIIIa. The catalogue of sources in declination range +30°. to +40°.
o	Table III: <Gra JHHMM+DDA> N=483.
=E=	Catalogue in electronic form as VIII/41
=E=	Catalogue in electronic form as VIII/80
Details on Acronym: [GRA2000]
[GRA2000]	(Georgelin+Russeil+Amram+, 2000)
Write:	<<[GRA2000] Complex LLL.l+B.b>> <<[GRA2000] HA LLL.l+B.b>> <<[GRA2000] CO LLL.l+B.bb>> <<[GRA2000] CO LLL.l+B.b>>
N:	22+7+2
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Table 1: col(1): N=22 HII region complexes, format 'Complex LLL.l+B.b', col(2): N=7 H-alpha emission sources, format 'HA LLL.l+B.b', col(3): N=2 CO em. sources, format 'CO LLL.l+B.bb' or 'CO LLL.l+B.b'. Paper V, see also [LAB92], [GAG94], [GRM96], [RGA98].
Ref:	=2000A&A...357..308G
by	GEORGELIN Y.M. , RUSSEIL D., AMRAM P., GEORGELIN Y.P., MARCELIN M., PARKER Q.A., VIALE A.
	Astron. Astrophys., 357, 308-324 (2000)
	Deep Hα survey of the Milky Way. V. The l=289° to 295° area.
o	Table 2, associated stars 'Br NN' from Brand thesis, 1986, Leiden, not in SIMBAD.
o	Table 1, col(1): <[GRA2000] Complex LLL.l+B.b> N=22. Table 1, col(2): <[GRA2000] HA LLL.l+B.b> N=7. Table 1, col(3): <[GRA2000] CO LLL.l+B.bb>, <[GRA2000] CO LLL.l+B.b> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Graff
Graff	(Graff)
Write:	<<Cl Graff N>>
N:	1
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Stat:	is completely incorporated in Simbad
Details on Acronym: Grah
Grah	(Graham)
*****	Avoid the usage of Grah, prefer [G81]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Graham
Graham	(Graham)
N:	1
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Stat:	is completely incorporated in Simbad
Details on Acronym: Gran
Gran	(Gran)
Write:	<<Gran N>>
N:	5
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	N=5 globular clusters towards the Galactic bulge. Use of Gaia DR2 and EDR3 data, and VVV data.
Ref:	=2019A&A...628A..45G
by	GRAN F. , ZOCCALI M., CONTRERAS RAMOS R., VALENTI E., ROJAS-ARRIAGADA A., CARBALLO-BELLO J.A., ALONSO-GARCIA J., MINNITI D., REJKUBA M., SUROT F.
	Astron. Astrophys., 628A, 45-45 (2019)
	Globular cluster candidates in the Galactic bulge: Gaia and VVV view of the latest discoveries.
o	Fig. 1, Table 1: <Gran 1> N=1.
Ref:	=2022MNRAS.509.4962G
by	GRAN F. , ZOCCALI M., SAVIANE I., VALENTI E., ROJAS-ARRIAGADA A., CONTRERAS RAMOS R., HARTKE J., CARBALLO-BELLO J.A., NAVARRETE C., REJKUBA M., OLIVARES CARVAJAL J.
	Mon. Not. R. Astron. Soc., 509, 4962-4981 (2022)
	Hidden in the haystack: low-luminosity globular clusters towards the Milky Way bulge.
o	Table 1: <Gran N> (Nos 2-5), <[GZS2022] C1> N=1.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Granat
Granat	(Granat satellite)= (GRS)
Write:	<<Granat HHMM+DD>> <<Granat HHMM+DDd>> <<Granat HHMM.m+DDMM>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	1st reference from this satellite (usually found as GRS in the literature). In this ref., N=1 (X) source.
Ref:	=1990IAUC.5032....1M
by	MANDROU P.
	IAU Circ., 5032, 1-None (1990)
	Galactic Center.
o	First ref. from this satellite. In this ref. <Granat HHMM+DDd> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Grasdalen
Grasdalen	(Discoverer: Grasdalen)
N:	1
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Stat:	is completely incorporated in Simbad
Ref:	=1975ApJ...197...77V
by	VRBA F.J. , STROM K.M., STROM S.E., GRASDALEN G.L.
	Astrophys. J., 197, 77-84 (1975)
	Futher study of the stellar cluster embedded in the Ophiuchus dark cloud complex.
o	Table 1: <VSSG NN> (Nos 1-31). <NAME GRASDALEN CL>
Details on Acronym: GRB
GRB	(Gamma Ray Burst)
*****	Avoid the usage of GRB, prefer 1B
Origin	of the Acronym: L = Found in the literature
Details on Acronym: GRB
GRB	(Gamma Ray Burst)
*****	Avoid the usage of GRB, prefer 2B
Origin	of the Acronym: L = Found in the literature
Details on Acronym: GRB
GRB	(Gamma Ray Burst)
*****	Avoid the usage of GRB, prefer 3B
Origin	of the Acronym: L = Found in the literature
Details on Acronym: GRB
GRB	(Gamma Ray Burst)
*****	Avoid the usage of GRB, prefer 4B
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Grb
Grb	(Groombridge)
*****	Avoid the usage of Grb, prefer Gmb
Details on Acronym: GRB
GRB	(Gamma-Ray Burst)= GB = (GRBS) = (SHB)
Write:	<<GRB YYMMDDA>> <<GRB YYMMDDa>> (not recognised by Simbad, but found in literature)
Object:	(Gamma) (SIMBAD class: gammaBurst = Gamma-ray Burst)
Note:	Systematic designation. The authors use 2 formats: 'YYMMDDA' or 'YYYY MMM DDA' for Year, Month and Day. A letter is added when several events have occured on the same day, the letter 'A' to the brightest burst. Only the first two references are given here: 1982ApJ...259L..51K: N=95 1987ApJS...64..305A: N=84
Ref:	=1982ApJ...259L..51K
by	KLEBESADEL R. , EVANS W.D., LAROS J.G., STRONG I.B., CLINE T.L., DESAI U., TEEGARDEN B.J., BARAT C., HURLEY K., NIEL M., VEDRENNE G., ESTULIN I.V., KUZNETSOV A.V., ZENCHENKO V.M.
	Astrophys. J., 259, 51-56 (1982)
	A catalog of γ-ray bursts with Earth crossing times.
o	<GRB YYMMDDA> N=111, <GBS HHMM+DD> N=16
Ref:	=1987ApJS...64..305A
by	ATTEIA J.L. , BARAT C., HURLEY K., NIEL M., VEDRENNE G., EVANS W.D., FENIMORE E.E., KLEBESADEL R.W., LAROS J.G., CLINE T., DESAI U., TEEGARDEN B., ESTULIN I.V., ZENCHENKO V.M., KUZNETSOV A.V., KURT V.G.
	Astrophys. J., Suppl. Ser., 64, 305-382 (1987)
	A second catalog of γ-ray bursts : 1978-1980 localizations from the interplanetary network.
o	Table 1: <[ABH87] NN> (Nos 1-84) = <GRB YYMMDDA> N=84.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GRB2005]
[GRB2005]	(Gratadour+Rouan+Boccaletti+, 2005) (Not yet in Simbad)
Write:	<<[GRB2005] Spot AN>> <<[GRB2005] Knot IR-Na>>
N:	2+7+2
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Observations of the nucleus of NGC 1068 at Ks with NAOS-CONICA at the VLT.
in source:	NGC 1068
Ref:	=2005A&A...429..433G
by	GRATADOUR D. , ROUAN D., BOCCALETTI A., RIAUD P., CLENET Y.
	Astron. Astrophys., 429, 433-437 (2005)
	Four quadrant phase mask K-band coronagraphy of NGC 1068 with NAOS-CONICA at VLT.
o	Figs: <[GRB2005] Spot AN> (Nos N1, N2), <[GRB2005] Knot IR-N> (Nos 1-4).
Ref:	=2006A&A...446..813G
by	GRATADOUR D. , ROUAN D., MUGNIER L.M., FUSCO T., CLENET Y., GENDRON E., LACOMBE F.
	Astron. Astrophys., 446, 813-825 (2006)
	Near-infrared adaptive optics dissection of the core of NGC 1068 with NAOS-CONICA.
o	fig. 4, Tables 1-2: <[GRB2005] Knot IR-Na> (Nos 6, 1a-1b) added, <[GRB2005] Source CW> (Nos CN, CS).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GRBS
GRBS	(Gamma Ray Burst Source)
*****	Avoid the usage of GRBS, prefer GRB
Details on Acronym: [GRC2000]
[GRC2000]	(Girart+Rodriguez+Curiel, 2000)= (VLA)
Write:	<<[GRC2000] VLA N>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
in source:	NAME RHO OPH CLOUD:YLW 15 = YLW 15
Ref:	=2000ApJ...544L.153G
by	GIRART J.M. , RODRIGUEZ L.F., CURIEL S.
	Astrophys. J., 544, 153-156 (2000)
	A subarcsecond binary radio source associated with the X-ray-emitting young stellar object YLW 15.
o	Table 1, Fig.1: <[GRC2000] VLA N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRC2002]
[GRC2002]	(Giavalisco+Riess+Casertano+, 2002)
Write:	<<[GRC2002] JHHMMSS.ss+DDMMSS.ss>>
N:	4
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxies of SN 2002FW, SN 2002FX, SN 2002FZ and SN 2002GA.
Ref:	=2002IAUC.7981....1G
by	GIAVALISCO M. , RIESS A., CASERTANO S., DAHLEN T., DICKINSON M., FERGUSON H., HOOK R., IDZI R., KOEKEMOER A., MOBASHER B., MOUSTAKAS L.A., RAVINDRANATH S., STROLGER L., TONRY J., CHALLIS P.
	IAU Circ., 7981, 1-None (2002)
	Supernovae 2002ez, 2002fv, 2002fw, 2002fx, 2002fy, 2002fz, 2002ga.
o	<[GRC2002] JHHMMSS.ss+DDMMSS.ss> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRC90]
[GRC90]	(Gyulbudaghian+Rodriguez+Curiel, 1990)
Write:	<<[GRC90] BHHMMSS.s+DDMMSS>> <<[GRC90] IRAS 21144+5430 N>>
N:	9+8
Object:	H2O Maser + (Rad) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Search for H2O masers in IRAS sources. 9 are detected in Haystack observations. In IRAS 21144+5430 N=8 6cm continuum emission sources detected in follow-up VLA observations.
in source:	IRAS 21144+5430
in source:	IRAS 21173+5450
in source:	IRAS 21368+5456
in source:	IRAS 21388+5622
in source:	IRAS 21391+5802
in source:	IRAS 21413+5442
in source:	IRAS 21479+5510
in source:	IRAS 21542+5558
in source:	IRAS 21561+5806
Ref:	=1990RMxAA..20...51G
by	GYULBUDAGHIAN A.L. , RODRIGUEZ L.F., CURIEL S.
	Rev. Mex. Astron. Astrofis., 20, 51-None (1990)
	New H2O masers in color-selected IRAS point sources.
o	Table 1: <[GRC90] BHHMMSS.s+DDMMSS> N=9. Table 2: <[GRC90] IRAS 21144+5430 N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: grCS
grCS	(g-r Color Selected) (Not yet in Simbad)
Write:	<<grCS NNN>>
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	In preparation. g-r Colour Selected. Clusters detected as localized overdensities of galaxies of a given colour in the XMM-LSS sky region. See also JKCS, RzCS, zKCS. The list of a few public clusters is at: http://www.brera.mi.astro.it/~andreon/clusters_p_ublic.html.
Auth.:	ANDREON S.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [GRD2007]
[GRD2007]	(Garay+Rodriguez+De Gregorio-Monsalvo, 2007)
Write:	<<[GRD2007] HHMMm+DDMMA>>
N:	5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 7mm observations toward 3 massive star-forming regions.
in source:	IRAS 18470-0044
in source:	IRAS 19217+1651
in source:	IRAS 23151+5912
Ref:	=2007AJ....134..906G
by	GARAY G. , RODRIGUEZ L.F., DE GREGORIO-MONSALVO I.
	Astron. J., 134, 906-911 (2007)
	Very large array observations of candidate high-mass protostellar objects at 7 millimeters.
o	Calibrator J1851+005 not identified (could be VCS2 J1851+0035?)
o	Tables 2, 3, Figs 1, 2: <[GRD2007] HHMMm+DDMMA> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GRDG
GRDG	(G. Reaves, Dwarf G)= (GR) = (G.R.)
Write:	<<GRDG NN>> <<GRDG +DD NNN>>
N:	846+90
Object:	Dwarf G (SIMBAD class: Galaxy)
Note:	Format 'NN' (Nos 1-91), No. 83 missing, (Nos 1-66) in 1956AJ.....61...69R, (Nos 67-82) in Reaves Thesis 1952, Univ. of California, Berkeley, (Nos 84-90) in 1962PASP...74..392R, No. 91 in Tinsley + Larson (New Haven: Yale Univ. Obs.) p. 39. Format '+DD NNN', N=846, in 1983ApJS...53..375R.
in source:	NAME Virgo Cluster
Ref:	=1956AJ.....61...69R
by	REAVES G.
	Astron. J., 61, 69-76 (1956)
	Dwarf galaxies in the Virgo cluster.
o	Tables I and II: <GRDG NN> (Nos 1-66).
Ref:	=1962PASP...74..392R
by	REAVES G.
	Publ. Astron. Soc. Pac., 74, 392-397 (1962)
	Dwarf galaxies in Virgo cluster.
o	Table I: <GRDG NN> (Nos 84-90) No. 91 is in Reaves, 1977 publication
Ref:	=1983ApJS...53..375R
by	REAVES G.
	Astrophys. J., Suppl. Ser., 53, 375-395 (1983)
	A catalog of dwarf galaxies in Virgo.
o	Table 2: <GRDG +DD NN> N=846
Details on Acronym: [GRE2009]
[GRE2009]	(Girart+Rao+Estalella, 2009)
Write:	<<[GRE2009] SMA N>>
N:	2
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	Submillimeter Array (SMA) 1.35mm observations of the field of IRAS 19156+1906.
in source:	LDN 723
Ref:	=2009ApJ...694...56G
by	GIRART J.M. , RAO R., ESTALELLA R.
	Astrophys. J., 694, 56-68 (2009)
	The L723 low-mass star forming protostellar system: resolving a double core.
o	Table 2: <[GRE2009] SMA N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRF2004]
[GRF2004]	(Guainazzi+Rodriguez-Pascual+Fabian+, 2004)
Write:	<<[GRF2004] NGC 5643 X-1>> <<[GRF2004] JHHMMSS.s+DDMMSS>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observation of NGC 5643: One source, [GRF2004] NGC 5643 X-1 coincides with the nucleus of NGC 5643, the other at about 0.8arcmin north-east of the nucleus is two times brighter than the nucleus.
in source:	NGC 5643
Ref:	=2004MNRAS.355..297G
by	GUAINAZZI M. , RODRIGUEZ-PASCUAL P., FABIAN A.C., IWASAWA K., MATT G.
	Mon. Not. R. Astron. Soc., 355, 297-306 (2004)
	Unveiling the nature of the highly obscured active galactic nucleus in NGC 5643 with XMM-Newton.
o	Text, Table 5: <[GRF2004] NGC 5643 X-1> N=1, <[GRF2004] JHHMMSS.s+DDMMSS> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GRG
GRG	(Khabibullina+Verkhodanov+Singh+, 2010)
*****	Avoid the usage of GRG, prefer [KVS2010]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GRG
GRG	(Khabibullina+Verkhodanov+Singh+, 2011)
*****	Avoid the usage of GRG, prefer [KVS2011]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GRG2000]
[GRG2000]	(Gomez+Rodriguez+Garay, 2000)= (VLA)
Write:	<<[GRG2000] VLA NN>>
N:	10
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
in source:	NAME GGD 12-15
Ref:	=2000ApJ...531..861G
by	GOMEZ Y. , RODRIGUEZ L.F., GARAY G.
	Astrophys. J., 531, 861-867 (2000)
	A cluster of radio sources near GGD 14.
o	Table 1: <[GRG2000] VLA N> (Nos 1-7).
Ref:	=2002ApJ...571..901G
by	GOMEZ Y. , RODRIGUEZ L.F., GARAY G.
	Astrophys. J., 571, 901-905 (2002)
	The nature of the cluster of radio sources in GGD 14.
o	Table 1: <[GRG2000] VLA NN> (Nos 8-10) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRG2003]
[GRG2003]	(Gomez+Rodriguez+Girat+, 2003)
Write:	<<[GRG2003] WW>> <<[GRG2003] H2O maser>> <<[GRG2003] mm>>
N:	3+1+1
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	VLA observations. N=3 molecular NH3 components in the HH 80-81 system, N=1 H2O maser and N=1 mm peak.
in source:	NAME HH 80-81
Ref:	=2003ApJ...597..414G
by	GOMEZ Y. , RODRIGUEZ L.F., GIRART J.M., GARAY G., MARTI J.
	Astrophys. J., 597, 414-423 (2003)
	VLA and BIMA observations toward the exciting source of the massive HH 80-81 outflow.
o	Fig.4, Table 3: <[GRG2003] WW> (Nos C, NE, S). Fig.2: <[GRG2003] H2O maser> N=1, <[GRG2003] mm> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRG2014]
[GRG2014]	(Greggio+Rejkuba+Gonzalez+, 2014)
Write:	<<[GRG2014] JHHMMSS.sss+DDMMSS.ss>>
N:	82712
Object:	* (SIMBAD class: Star)
Note:	VISTA VIRCAM observations of the stellar halo of NGC 253.
in source:	NGC 253
Ref:	=2014A&A...562A..73G
by	GREGGIO L. , REJKUBA M., GONZALEZ O.A., ARNABOLDI M., IODICE E., IRWIN M., NEESER M.J., EMERSON J.
	Astron. Astrophys., 562A, 73-73 (2014)
	A panoramic VISTA of the stellar halo of NGC 253.
o	Catalog B: <[GRG2014] JHHMMSS.sss+DDMMSS.ss> N=82712.
=E=	Catalogue in electronic form as J/A+A/562/A73
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GRH
GRH	(Gilmore+Reid+Hewett)
Write:	<<GRH HHMMSS.s+DDMMSS>>
N:	24
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1985MNRAS.213..257G
by	GILMORE G. , REID N., HEWETT P.
	Mon. Not. R. Astron. Soc., 213, 257-278 (1985)
	New light on faint stars - VII. Luminosity and mass distributions in two high galactic latitude fields.
o	Appendix A: <GRH HHMMSS.s-DDMMSS> N=24
Origin	of the Acronym: L (1996MNRAS.281..644T)
Details on Acronym: [GRH2022]
[GRH2022]	(Garcia-Vergara+Rybak+Hodge+, 2022)
Write:	<<[GRH2022] JHHMM+DDMM.N>>
N:	9
Object:	Em. G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 3 observations of N=9 emission-line galaxies in the fields of eight quasars.
Ref:	=2022ApJ...927...65G
by	GARCIA-VERGARA C. , RYBAK M., HODGE J., HENNAWI J.F., DECARLI R., GONZALEZ-LOPEZ J., ARRIGONI-BATTAIA F., ARAVENA M., FARINA E.P.
	Astrophys. J., 927, 65-65 (2022)
	ALMA Reveals a Large Overdensity and Strong Clustering of Galaxies in Quasar Environments at z ~ 4.
o	Fig. 2, Table 3: <[GRH2022] JHHMM+DDMM.N> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Gri
Gri	(Grindlay)
Write:	<<NAME Gri N>>
N:	1
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Rem:	= C 1728-338
Ref:	=1981ApJ...247L..17G
by	GRINDLAY J.E. , HERTZ P.
	Astrophys. J., 247, 17-21 (1981)
	Discovery of an obscured globular cluster associated with GX 354+0 (=4U/MXB 1728-34).
o	<NAME Gri N> N=1
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GRK2002]
[GRK2002]	(Goad+Roberts+Knigge+, 2002)
Write:	<<[GRK2002] HST N>>
N:	3
Object:	? (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Archival HST/WFPC2 images are used to search for possible optical counterparts of [RW2000] NGC 5204 X-1. See also [RGW2001].
in source:	NGC 5204
Ref:	=2002MNRAS.335L..67G
by	GOAD M.R. , ROBERTS T.P., KNIGGE C., LIRA P.
	Mon. Not. R. Astron. Soc., 335, 67-70 (2002)
	The optical counterpart of the ultraluminous X-ray source NGC 5204 X-1.
o	Fig.1, Table 1: <[GRK2002] HST N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRL2000]
[GRL2000]	(Giovanardi+Rodriguez+Lizano+, 2000)
Write:	<<[GRL2000] NN>>
N:	26
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=26 21cm continuum sources in the field of LDN 1551.
in source:	LDN 1551
Ref:	=2000ApJ...538..728G
by	GIOVANARDI C. , RODRIGUEZ L.F., LIZANO S., CANTO J.
	Astrophys. J., 538, 728-737 (2000)
	Very large array observations of high-velocity H I in L1551.
o	Table 1: <[GRL2000] NN> (Nos 1-26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRL91]
[GRL91]	(Gallais+Rouan+Lacombe+, 1991)= (Gallais)
Write:	<<[GRL91] N>>
N:	7
Object:	Region (SIMBAD class: Region = Region defined in the Sky)
Stat:	is completely incorporated in Simbad
in source:	M 83 = NGC 5236
Ref:	=1991A&A...243..309G
by	GALLAIS P. , ROUAN D., LACOMBE F., TIPHENE D., VAUGLIN I.
	Astron. Astrophys., 243, 309-None (1991)
	The nuclear starburst activity in M 83 : imaging at near-IR wavelengths.
o	Table 4: <[GRL91] N> N=7
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GRM
GRM	(Gomez+Rodriguez+Mirabel)
Write:	<<GRM N>>
N:	3
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Radio observations of 3 objects: see [GRM97]. 2 are possible PN, 1 is a possible HII region, the 3 are identified as PN in the first suppl. of Strasbourg-ESO catalogue of galactic PN.
Ref:	=1997RMxAA..33...25G
by	GOMEZ Y. , RODRIGUEZ L.F., MIRABEL I.F.
	Rev. Mex. Astron. Astrofis., 33, 25-30 (1997)
	Candidate planetary nebulae near the Galactic Center.
o	Table 1: <GRM N> (Nos 1-3) = <[GRM97] GLLL.lll-B.bbb> N=3.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Grm
Grm	(?)
*****	Avoid the usage of Grm, prefer MCL
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GRM2013]
[GRM2013]	(Geier+Richard+Man+, 2013)
Write:	<<[GRM2013] A1413-1>> <<[GRM2013] MACS2129-1>>
N:	2
Object:	Grav. lensed image of a G (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT X-Shooter spectroscopic observations of N=2 gravitationally lensed distant massive quiescent galaxies.
Ref:	=2013ApJ...777...87G
by	GEIER S. , RICHARD J., MAN A.W.S., KRUHLER T., TOFT S., MARCHESINI D., FYNBO J.P.U.
	Astrophys. J., 777, 87 (2013)
	VLT/X-shooter near-infrared spectroscopy and HST imaging of gravitationally lensed z ~ 2 compact quiescent galaxies.
o	Table 1: <[GRM2013] A1413-1>, <[GRM2013] MACS2129-1>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRM2014]
[GRM2014]	(Graur+Rodney+Maoz+, 2014)
Write:	<<[GRM2014] CLAYYAaa>> <<[GRM2014] CLAYYAaa Host G>>
N:	27+27
Object:	SN + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Keck I and II (LRIS and DEIMOS), Gemini GMOS, LBT MODS, VLT (FORS, VIMOS, X-Shooter) spectroscopy of N=27 supernova candidates discovered in the CLASH program. The format of the SN Designation is based on the cluster and year in which they were discovered and the first three letters of the nickname given to them for internal tracking purposes. For example, CLI11Had is a CLASH (CL) SN that was discovered in one of the parallel fields around the ninth (or Ith) cluster (MCS J0717.5+3745), in 2011, and was nicknamed "Hadrian".
Ref:	=2014ApJ...783...28G
by	GRAUR O. , RODNEY S.A., MAOZ D., RIESS A.G., JHA S.W., POSTMAN M., DAHLEN T., HOLOIEN T.W.-S., McCULLY C., PATEL B., STROLGER L.-G., BENITEZ N., COE D., JOUVEL S., MEDEZINSKI E., MOLINO A., NONINO M., BRADLEY L., KOEKEMOER A., BALESTRA I., CENKO S.B., CLUBB K.I., DICKINSON M.E., FILIPPENKO A.V., FREDERIKSEN T.F., GARNAVICH P., HJORTH J., JONES D.O., LEIBUNDGUT B., MATHESON T., MOBASHER B., ROSATI P., SILVERMAN J.M., U V., JEDRUSZCZUK K., LI C., LIN K., MIRMELSTEIN M., NEUSTADT J., OVADIA A., ROGERS E.H.
	Astrophys. J., 783, 28 (2014)
	Type-Ia supernova rates to redshift 2.4 from CLASH: the cluster lensing and supernova survey with Hubble.
o	Table 2: <[GRM2014] CLAYYAaa> N=27, <[GRM2014] CLAYYAaa Host G> N=27.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRM93]
[GRM93]	(Garay+Rodriguez+Moran+, 1993)
Write:	<<[GRM93] GLL.ll+B.bb A>> <<[GRM93] GLL.ll+B.bb AN>> <<[GRM93] GLL.ll+B.bb AA>>
N:	30
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	In the format 'GLL.ll+B.bb AN' or 'GLL.ll+B.bb AA', the letter 'G' stands for Galactic coordinates, the objects 'GAL LL.ll+B.bb' are HII regions.
Ref:	=1993ApJ...418..368G
by	GARAY G. , RODRIGUEZ L.F., MORAN J.M., CHURCHWELL E.
	Astrophys. J., 418, 368-385 (1993)
	VLA observations of strong IRAS point sources associated with compact H II regions.
o	Tables 2, 3: <[GRM93] GLL.ll+B.bb AN> and <[GRM93] GLL.ll+B.bb AA>, N=21
Ref:	=1996ApJ...460..359H
by	HOFNER P. , KURTZ S., CHURCHWELL E., WALMSLEY C.M., CESARONI R.
	Astrophys. J., 460, 359-371 (1996)
	Massive star formation in the hot, dense cloud core of G9.62+0.19.
o	Table 2: Components D, E, F in G9.62+0.19 = [GRM93]
o	Table 2: <[GRM93] G9.61+0.20 A> (No. F) added.
Ref:	=2000A&A...359L...5T
by	TESTI L. , HOFNER P., KURTZ S., RUPEN M.
	Astron. Astrophys., 359, 5-8 (2000)
	Detection of the thermal radio continuum emission from the G9.62+0.19-F hot core.
o	Table 2: <[GRM93] G9.61+0.20 A> (Nos G-I) added.
Ref:	=2001ApJ...549..425H
by	HOFNER P. , WIESEMEYER H., HENNING T.
	Astrophys. J., 549, 425-432 (2001)
	A high-velocity molecular outflow from the G9.62+0.19 star-forming region.
o	Figs: <[GRM93] G9.61+0.20 A> (No. J) added.
Ref:	=2005A&A...429..903L
by	LINZ H. , STECKLUM B., HENNING T., HOFNER P., BRANDL B.
	Astron. Astrophys., 429, 903-921 (2005)
	The G9.62+0.19-F hot molecular core. The infrared view on very young massive stars.
o	G9.62+0.19-F = [GRM93] G09.61+0.20 F in SIMBAD.
o	Table 2: <[GRM93] G09.61+0.20 AN> (Nos F1-F4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRM95]
[GRM95]	(Gomez+Rodriguez+Marti, 1995)= (VLA)
Write:	<<[GRM95] VLA N>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=3 'VLA N' (Nos 1-3)
in source:	NAME HH 80-81
Ref:	=1995ApJ...453..268G
by	GOMEZ Y. , RODRIGUEZ L.F., MARTI J.
	Astrophys. J., 453, 268-270 (1995)
	Thermal jets and H2O masers : the case of HH 80-81.
o	T.1: SC = [MRR95] SC
o	Table 1: <[GRM95] VLA N> (Nos 1-3)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRM96]
[GRM96]	(Georgelin+Russeil+Marcelin+, 1996)
Write:	<<[GRM96] LLL.lll+B.bbb>> <<[GRM96] LLL.l+B.b>> <<[GRM96] CO HHMM+DDMM>> <<[GRM96] DC LLL.l+B.b>>
N:	39+1+7
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Table 2: HII region complexes. N=39 radio continuum sources, format 'LLL.lll+B.bbb' or 'LLL.l+B.b'. N=7 Dark Cloud, format 'DC LLL.l+B.b'. N=1 CO em. source, format 'CO HHMM+DDMM'. Paper III, see also [LAB92], [GAG94], [RGA98], [GRA2000].
Ref:	=1996A&AS..120...41G
by	GEORGELIN Y.M. , RUSSEIL D., MARCELIN M., AMRAM P., GEORGELIN Y.P., GOLDES G., LE COARER E., MORANDINI M.
	Astron. Astrophys., Suppl. Ser., 120, 41-56 (1996)
	Deep Hα survey of the Milky Way. III. The l=338° area.
o	Table 2: <[GRM96] LLL.lll+B.bbb>, <[GRM96] LLL.l+B.b> N=39, <[GRM96] CO HHMM+DDMM> N=1, <[GRM96] DC LLL.l+B.b> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRM97]
[GRM97]	(Gomez+Rodriguez+Mirabel, 1997)
Write:	<<[GRM97] GLLL.lll-B.bbb>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio observations of 3 objects: 2 are possible PN, 1 is a possible HII region. The 3 objects are confirmed as PN in the literature. See also GRM.
Ref:	=1997RMxAA..33...25G
by	GOMEZ Y. , RODRIGUEZ L.F., MIRABEL I.F.
	Rev. Mex. Astron. Astrofis., 33, 25-30 (1997)
	Candidate planetary nebulae near the Galactic Center.
o	Table 1: <GRM N> (Nos 1-3) = <[GRM97] GLLL.lll-B.bbb> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Grn
Grn	(Groningen obs.)
*****	Avoid the usage of Grn, prefer BSD
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GRN94]
[GRN94]	(Griffiths+Ratnatunga+Neuschaefer+, 1994)= (HST) = (MDS)
Write:	<<[GRN94] A>> <<[GRN94] JHHMMSS.ss+DDMMSS.s>>
N:	143
Object:	G (SIMBAD class: Galaxy)
Note:	Fig. 3 and p. 74: (Nos A-F). Tables 3A-3D: N=143, including 23 stars and 2 other objects, in the field of 3C 273, format 'JHHMMSS.ss+DDMMSS.s'. HST Medium Deep Survey, WFC and PC. Maps: plates 3-4
Ref:	=1994ApJ...437...67G
by	GRIFFITHS R.E. , RATNATUNGA K.U., NEUSCHAEFER L.W., CASERTANO S., IM M., WYCKOFF E.W., ELLIS R.S., GILMORE G.F., ELSON R.A.W., GLAZEBROOK K., SCHADE D.J., WINDHORST R.A., SCHMIDTKE P.C., GORDON J.M., PASCARELLE S.M., ILLINGWORTH G.D., KOO D.C., BERSHADY M.A., FORBES D.A., PHILLIPS A.C., GREEN R.F., SARAJEDINI V., HUCHRA J.P., TYSON A.J.
	Astrophys. J., 437, 67-82 (1994)
	The Hubble Space Telescope Medium Deep Survey with the Wide Field and Planetary Camera. I. Methodology and results on the field near 3C 273.
o	p. 74: <[GRN94] A> (Nos A-F), Tables 3A-3D: <[GRN94] JHHMMSS.ss+DDMMSS.s> N=143
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GRO
GRO	(Gamma Ray Observatory)= CGRO
Write:	<<GRO JHHMM+DD>> <<GRO JHHMM+DDd>>
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	1st reference from this satellite. In this ref., N=1 (Gamma) source.
Ref:	=1992IAUC.5584....1H
by	HARMON B.A. , WILSON R.B., FISHMAN G.J., MEEGAN C.A., PACIESAS W.S., BRIGGS M.S., FINGER M.H., CAMERON R., KROEGER R., GROVE E.
	IAU Circ., 5584, 1-None (1992)
	GRO J0422+32.
o	<GRO JHHMM+DD> N=1.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Groombridge
Groombridge	(Groombridge)
====>	Equivalent to: Gmb
Details on Acronym: Groth
Groth	(Groth strip survey)
*****	Avoid the usage of Groth, prefer DEEP-GSS
Origin	of the Acronym: L (2003ApJ...597..239G)
Details on Acronym: Group
Group	(Group of G)
*****	Avoid the usage of Group, prefer [FWB89]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GRP2019]
[GRP2019]	(Gomez-Guijarro+Riechers+Pavesi+, 2019)
Write:	<<[GRP2019] HCOSMOS02-SNN>>
N:	10
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA band 3 (3mm), VLA 12CO(1-0), CARMA 12CO(3-2), and NOEMA 12CO(4-3) observations of N=10 sources in the field of 1HERMES S250 J100056.6+022014 (HCOSMOS02).
Ref:	=2019ApJ...872..117G
by	GOMEZ-GUIJARRO C. , RIECHERS D.A., PAVESI R., MAGDIS G.E., LEUNG T.K.D., VALENTINO F., TOFT S., ARAVENA M., CHAPMAN S.C., CLEMENTS D.L., DANNERBAUER H., OLIVER S.J., PEREZ-FOURNON I., VALTCHANOV I.
	Astrophys. J., 872, 117-117 (2019)
	Confirming Herschel candidate protoclusters from ALMA/VLA CO observations.
o	Figs 5-6, Table 4: <[GRP2019] HCOSMOS02-SNN> (Nos S5-S14).
o	GOODS-N at z=1.99 and COSMOS at z=2.10 and z=2.51 protoclusters, as well as COSMOS overdensity are not in SIMBAD.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRR2001]
[GRR2001]	(Gosset+Royer+Rauw+, 2001) (Not yet in Simbad)
Write:	<<[GRR2001] A>>
N:	8
Object:	* (SIMBAD class: Star)
Note:	N=8 comparison stars in the finding chart of WR 30a.
Ref:	=2001MNRAS.327..435G
by	GOSSET E. , ROYER P., RAUW G., MANFROID J., VREUX J.-M.
	Mon. Not. R. Astron. Soc., 327, 435-451 (2001)
	A first detailed study of the colliding wind WR+O binary WR 30a.
o	Fig.1: <[GRR2001] A> (Nos A-H).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRR96]
[GRR96]	(Garay+Ramirez+Rodriguez+, 1996)
Note:	Table 5
*****	Avoid the usage of [GRR96], prefer [HM90]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GRRV
GRRV	(Glass+Reid, Red Variable)= (GR) = (LMC VAR)
Write:	<<GRRV NN>>
N:	49
Object:	Red V* (SIMBAD class: Variable* = Variable Star)
Note:	UK Schmidt-based V-and I-band photographic survey for large-amplitude red variable stars in a field of the LMC. Infrared JHK photometry.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1985MNRAS.214..405G
by	GLASS I.S. , REID N.
	Mon. Not. R. Astron. Soc., 214, 405-418 (1985)
	A survey for red variables in the LMC I.
o	Table 2: <GRRV NN> (Nos 1-49)
Details on Acronym: GRS
GRS	(Globule of Radial Systems)
*****	Avoid the usage of GRS, prefer [G85]
Details on Acronym: GRS
GRS	(Granat Source)
*****	Avoid the usage of GRS, prefer Granat
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GRS
GRS	(Gal. Radio Source)= (G)
Write:	<<GRS GLLL.l+BB.b>> <<GRS GLLL.ll+BB.bb>>
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Systematic designation
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRS2000]
[GRS2000]	(Germany+Reiss+Sadler+, 2000) (Not yet in Simbad)
Write:	<<[GRS2000] NN>>
N:	10
Object:	* (SIMBAD class: Star)
Note:	N=10 reference stars in the field of SN 1997CY. Identif. chart fig.1
Ref:	=2000ApJ...533..320G
by	GERMANY L.M. , REISS D.J., SADLER E.M., SCHMIDT B.P., STUBBS C.W.
	Astrophys. J., 533, 320-328 (2000)
	SN 1997cy/GRB 970514: a new piece in the γ-ray burst puzzle ?
o	Table 1: <[GRS2000] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRS2009]
[GRS2009]	(Guieu+Rebull+Stauffer+, 2009)= ([GRS2009a])
Write:	<<[GRS2009] N>> <<[GRS2009] SST JHHMMSS.s+DDMMSS.s>>
N:	8+1657
Object:	Cluster of * + Y*? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC observations of the North America and Pelican nebulae.
in source:	NGC 7000 = NAME North America Nebula
in source:	IC 5070 = NAME Pelican Nebula
Ref:	=2009ApJ...697..787G
by	GUIEU S. , REBULL L.M., STAUFFER J.R., HILLENBRAND L.A., CARPENTER J.M., NORIEGA-CRESPO A., PADGETT D.L., COLE D.M., CAREY S.J., STAPELFELDT K.R., STROM S.E.
	Astrophys. J., 697, 787-800 (2009)
	The North American and Pelican nebulae. I. IRAC observations.
o	Table 3: <[GRS2009] N> (Nos 1-8). Table 4: <[GRS2009] SST JHHMMSS.s+DDMMSS.s> N=1657.
=E=	Catalogue in electronic form as <J/ApJ/697/787/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRS2009a]
[GRS2009a]	(Guieu+Rebull+Stauffer+, 2009)
*****	Avoid the usage of [GRS2009a], prefer [GRS2009]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRS2009b]
[GRS2009b]	(Gaspar+Rieke+Su+, 2011)
Write:	<<[GRS2009b] NNN>>
N:	193
Object:	* (SIMBAD class: Star)
Note:	Spitzer MIPS observations at 24µm of the open cluster Praesepe.
in source:	NAME Praesepe
Ref:	=2009ApJ...697.1578G
by	GASPAR A. , RIEKE G.H., SU K.Y.L., BALOG Z., TRILLING D., MUZZEROLE J., APAI D., KELLY B.C.
	Astrophys. J., 697, 1578-1596 (2009)
	The low level of debris disk activity at the time of the late heavy bombardment: a Spitzer study of Praesepe.
o	Table 1: <[GRS2009b] NNN> (Nos 1-193).
=E=	Catalogue in electronic form as J/ApJ/697/1578
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRS2013]
[GRS2013]	(Goldman+Roeser+Schilbach+, 2013)= ([GRS2013a])
Write:	<<[GRS2013] NNNNNNNN>>
N:	62
Object:	* (SIMBAD class: Star)
Note:	Sample of N=62 Hyades candidate members. Use of PPMXL, SDSS DR8, UKIDSS DR8 and WISE data. See also [RSP2011].
in source:	Cl Melotte 25 = Hyades
Ref:	=2013A&A...559A..43G
by	GOLDMAN B. , ROESER S., SCHILBACH E., MAGNIER E.A., OLCZAK C., HENNING T., JURIC M., SCHLAFLY E., CHEN W.P., PLATAIS I., BURGETT W., HODAPP K., HEASLEY J., KUDRITZKI R.P., MORGAN J.S., PRICE P.A., TONRY J.L., WAINSCOAT R.
	Astron. Astrophys., 559A, 43-43 (2013)
	Towards a complete stellar mass function of the Hyades. I. Pan-STARRS1 optical observations of the low-mass stellar content.
o	<[GRS2013] NNNNNNNN> N=62 among (Nos 1221246-99624511).
=E=	Catalogue in electronic form as <J/A+A/559/A43/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRS2013a]
[GRS2013a]	(Goldman+Roeser+Schilbach+, 2013)
*****	Avoid the usage of [GRS2013a], prefer [GRS2013]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRS2013b]
[GRS2013b]	(Gladders+Rigby+Sharon+, 2013)
Write:	<<[GRS2013b] SDSS J1438+1454 system>> <<[GRS2013b] SDSS J1438+1454>> <<[GRS2013b] SDSS J1438+1454 BCG>>
N:	1+1+1
Object:	Grav. lens system + Grav. lens + Brightest Cluster Galaxy (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Magellan Baade telescope 6.5m FourStar and Gemini North, Herschel PACS and SPIRE, ARC 3.5m telescope DIS and Keck II NIRSPEC spectroscopy of N=1 gravitational lens system, N=1 gravitational lens, and N=1 brightest galaxy in the lensing cluster [GRS2013b] SDSS J1438+1454. Use of SDSS and Spitzer data.
Ref:	=2013ApJ...764..177G
by	GLADDERS M.D. , RIGBY J.R., SHARON K., WUYTS E., ABRAMSON L.E., DAHLE H., PERSSON S.E., MONSON A.J., KELSON D.D., BENFORD D.J., MURPHY D., BAYLISS M.B., FINKELSTEIN K.D., KOESTER B.P., BANS A., BAXTER E.J., HELSBY J.E.
	Astrophys. J., 764, 177 (2013)
	SGAS 143845.1+145407: a big, cool starburst at redshift 0.816.
o	<[GRS2013b] SDSS J1438+1454 system> N=1. <[GRS2013b] SDSS J1438+1454> N=1. <[GRS2013b] SDSS J1438+1454 BCG> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GRSMC
GRSMC	(Galactic Ring Survey, Molecular Cloud)
Write:	<<GRSMC LL.ll+B.bb>> <<GRSMC LL.lll+B.bbb>> <<GRSMC LL.ll+B.bb cNNN>>
N:	3+1+5+829+6124
Object:	MCld + Clump (SIMBAD class: MolCld = Molecular Cloud)
Note:	FCRAO 14m telescope 13CO(1-0) Milky Way galactic ring survey.
Ref:	=2001ApJ...551..747S
by	SIMON R. , JACKSON J.M., CLEMENS D.P., BANIA T.M., HEYER M.H.
	Astrophys. J., 551, 747-763 (2001)
	The structure of four molecular cloud complexes in the BU-FCRAO Milky Way galactic ring survey.
o	Table 1: <GRSMC LL.ll+B.bb> N=3.
Ref:	=2002ApJ...576..274M
by	McQUINN K.B.W. , SIMON R., LAW C.J., JACKSON J.M., BANIA T.M., CLEMENS D.P., HEYER M.H.
	Astrophys. J., 576, 274-284 (2002)
	A comparison of ^{13}CO and CS emission in the inner galaxy.
o	Fig.1: <GRSMC LL.ll+B.bb> (No. 45.70-0.40) added.
Ref:	=2003ApJ...588..918K
by	KRAEMER K.E. , JACKSON J.M., KASSIS M., DEUTSCH L.K., HORA J.L., SIMON R., HOFFMANN W.F., FAZIO G.G., DAYAL A., BANIA T.M., CLEMENS D.P., HEYER M.H.
	Astrophys. J., 588, 918-930 (2003)
	Five star-forming cores in the Galactic Ring Survey: a mid-infrared study.
o	Table 3: <GRSMC LL.lll+B.bbb> N=5 added. Table 3: <KJK G45.07 N> (Nos 1-3), <KJK G45.12 N> (Nos 1-2), <KJK G45.47 N> (Nos 1-2).
Ref:	=2009ApJS..182..131R
by	RATHBORNE J.M. , JOHNSON A.M., JACKSON J.M., SHAH R.Y., SIMON R.
	Astrophys. J., Suppl. Ser., 182, 131-142 (2009)
	Molecular clouds and clumps in the Boston University-Five College Radio Astronomy Observatory Galactic Ring Survey.
o	Table 2: <GRSMC LL.ll+B.bb> N=829. Table 3: <GRSMC LL.ll+B.bb cNNN> N=6124.
=E=	Catalogue in electronic form as J/ApJS/182/131
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Gru
Gru	(Grus) (Not yet in Simbad)
*****	Avoid the usage of Gru, prefer [CP83b]
Details on Acronym: GRV
GRV	(Glass+ Reid, Variable *)= (LMC R) = (NRV)
Write:	<<GRV HHMM+DDMM>>
N:	126
Object:	Red V* (SIMBAD class: Variable* = Variable Star)
Note:	see also SHV and RHV
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1988MNRAS.232...53R
by	REID N. , GLASS I.S., CATCHPOLE R.M.
	Mon. Not. R. Astron. Soc., 232, 53-79 (1988)
	A survey for red variables in the LMC. II.
o	Tables 4, 5: 1st col. <RGC NNN> N=126, 2nd col. <GRV HHMM-DDMM> N=126
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GRV
GRV	(Gyulbudaghian+Rodriguez+Villanueva)
*****	Avoid the usage of GRV, prefer [GRV93]
Origin	of the Acronym: L (1998Ap.....41..382G)
Details on Acronym: GRV
GRV	(Group of G, Vennik)
*****	Avoid the usage of GRV, prefer [V84]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GRV93]
[GRV93]	(Gyulbudaghian+Rodriguez+Villanueva, 1993)= (GRV)
Write:	<<[GRV93] NN>>
N:	23
Object:	Neb. Obj. (SIMBAD class: ISM = Interstellar Medium Object)
Stat:	is completely incorporated in Simbad
Note:	Plates for nebulous objects: Plates 1 to 5
Ref:	=1993RMxAA..25...19G
by	GYULBUDAGHIAN A.L. , RODRIGUEZ L.F., VILLANUEVA V.M.
	Rev. Mex. Astron. Astrofis., 25, 19-21 (1993)
	Nebulous objects on the ESO/SRC J plates.
o	<[GRV93] NN> (Nos 1-23).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Grw
Grw	(Greenwich obs.)
*****	Avoid the usage of Grw, prefer AC
Details on Acronym: GrW
GrW	(Gravitational Wave)= (GW)
Write:	<<GrW YYMMDDA>> <<GrW YYMMDD HHMMSS>> <<GrW YYMMDD_HHMMSS>> (not recognised by Simbad, but found in literature)
Object:	Grav. Wave Event (SIMBAD class: GravWaveEvent = Gravitational Wave Event)
Note:	Gravitational wave event detection. The first detections were made by the Laser Interferometer Gravitational-wave Observatory (LIGO). More information on the website: https://www.ligo.caltech.edu/
Ref:	=2016PhRvL.116f1102A
by	ABBOTT B.P. , ABBOTT R., ABBOTT T.D., ABERNATHY M.R., ACERNESE F., ACKLEY K., ADAMS C., ADAMS T., ADDESSO P., ADHIKARI R.X., ADYA V.B., AFFELDT C., AGATHOS M., AGATSUMA K., AGGARWAL N., AGUIAR O.D., AIELLO L., AIN A., AJITH P., ALLEN B., ALLOCCA A., ALTIN P.A., ANDERSON S.B., ANDERSON W.G., ARAI K., ARAIN M.A., ARAYA M.C., ARCENEAUX C.C., AREEDA J.S., ARNAUD N., ARUN K.G., ASCENZI S., ASHTON G., AST M., ASTON S.M., ASTONE P., AUFMUTH P., AULBERT C., BABAK S., BACON P., BADER M.K.M., BAKER P.T., BALDACCINI F., BALLARDIN G., BALLMER S.W., BARAYOGA J.C., BARCLAY S.E., BARISH B.C., BARKER D., BARONE F., BARR B., BARSOTTI L., BARSUGLIA M., BARTA D., BARTLETT J., BARTON M.A., BARTOS I., BASSIRI R., BASTI A., BATCH J.C., BAUNE C., BAVIGADDA V., BAZZAN M., BEHNKE B., BEJGER M., BELCZYNSKI C., BELL A.S., BELL C.J., BERGER B.K., BERGMAN J., BERGMANN G., BERRY C.P.L., BERSANETTI D., BERTOLINI A., BETZWIESER J., BHAGWAT S., BHANDARE R., BILENKO I.A., BILLINGSLEY G., BIRCH J., BIRNEY R., BIRNHOLTZ O., BISCANS S., BISHT A., BITOSSI M., BIWER C., BIZOUARD M.A., BLACKBURN J.K., BLAIR C.D., BLAIR D.G., BLAIR R.M., BLOEMEN S., BOCK O., BODIYA T.P., BOER M., BOGAERT G., BOGAN C., BOHE A., BOJTOS P., BOND C., BONDU F., BONNAND R., BOOM B.A., BORK R., BOSCHI V., BOSE S., BOUFFANAIS Y., BOZZI A., BRADASCHIA C., BRADY P.R., BRAGINSKY V.B., BRANCHESI M., BRAU J.E., BRIANT T., BRILLET A., BRINKMANN M., BRISSON V., BROCKILL P., BROOKS A.F., BROWN D.A., BROWN D.D., BROWN N.M., BUCHANAN C.C., BUIKEMA A., BULIK T., BULTEN H.J., BUONANNO A., BUSKULIC D., BUY C., BYER R.L., CABERO M., CADONATI L., CAGNOLI G., CAHILLANE C., CALDERON BUSTILLO J., CALLISTER T., CALLONI E., CAMP J.B., CANNON K.C., CAO J., CAPANO C.D., CAPOCASA E., CARBOGNANI F., CARIDE S., CASANUEVA DIAZ J., CASENTINI C., CAUDILL S., CAVAGLIA M., CAVALIER F., CAVALIERI R., CELLA G., CEPEDA C.B., CERBONI BAIARDI L., CERRETANI G., CESARINI E., CHAKRABORTY R., CHALERMSONGSAK T., CHAMBERLIN S.J., CHAN M., CHAO S., CHARLTON P., CHASSANDE-MOTTIN E., CHEN H.Y., CHEN Y., CHENG C., CHINCARINI A., CHIUMMO A., CHO H.S., CHO M., CHOW J.H., CHRISTENSEN N., CHU Q., CHUA S., CHUNG S., CIANI G., CLARA F., CLARK J.A., CLEVA F., COCCIA E., COHADON P.-F., COLLA A., COLLETTE C.G., COMINSKY L., CONSTANCIO M., CONTE A., CONTI L., COOK D., CORBITT T.R., CORNISH N., CORSI A., CORTESE S., COSTA C.A., COUGHLIN M.W., COUGHLIN S.B., COULON J.-P., COUNTRYMAN S.T., COUVARES P., COWAN E.E., COWARD D.M., COWART M.J., COYNE D.C., COYNE R., CRAIG K., CREIGHTON J.D.E., CREIGHTON T.D., CRIPE J., CROWDER S.G., CRUISE A.M., CUMMING A., CUNNINGHAM L., CUOCO E., DAL CANTON T., DANILISHIN S.L., D'ANTONIO S., DANZMANN K., DARMAN N.S., DA SILVA COSTA C.F., DATTILO V., DAVE I., DAVELOZA H.P., DAVIER M., DAVIES G.S., DAW E.J., DAY R., DE S., DEBRA D., DEBRECZENI G., DEGALLAIX J., DE LAURENTIS M., DELEGLISE S., DEL POZZO W., DENKER T., DENT T., DERELI H., DERGACHEV V., DEROSA R.T., DE ROSA R., DESALVO R., DHURANDHAR S., DIAZ M.C., DI FIORE L., DI GIOVANNI M., DI LIETO A., DI PACE S., DI PALMA I., DI VIRGILIO A., DOJCINOSKI G., DOLIQUE V., DONOVAN F., DOOLEY K.L., DORAVARI S., DOUGLAS R., DOWNES T.P., DRAGO M., DREVER R.W.P., DRIGGERS J.C., DU Z., DUCROT M., DWYER S.E., EDO T.B., EDWARDS M.C., EFFLER A., EGGENSTEIN H.-B., EHRENS P., EICHHOLZ J., EIKENBERRY S.S., ENGELS W., ESSICK R.C., ETZEL T., EVANS M., EVANS T.M., EVERETT R., FACTOUROVICH M., FAFONE V., FAIR H., FAIRHURST S., FAN X., FANG Q., FARINON S., FARR B., FARR W.M., FAVATA M., FAYS M., FEHRMANN H., FEJER M.M., FELDBAUM D., FERRANTE I., FERREIRA E.C., FERRINI F., FIDECARO F., FINN L.S., FIORI I., FIORUCCI D., FISHER R.P., FLAMINIO R., FLETCHER M., FONG H., FOURNIER J.-D., FRANCO S., FRASCA S., FRASCONI F., FREDE M., FREI Z., FREISE A., FREY R., FREY V., FRICKE T.T., FRITSCHEL P., FROLOV V.V., FULDA P., FYFFE M., GABBARD H.A.G., GAIR J.R., GAMMAITONI L., GAONKAR S.G., GARUFI F., GATTO A., GAUR G., GEHRELS N., GEMME G., GENDRE B., GENIN E., GENNAI A., GEORGE J., GERGELY L., GERMAIN V., GHOSH A., GHOSH A., GHOSH S., GIAIME J.A., GIARDINA K.D., GIAZOTTO A., GILL K., GLAEFKE A., GLEASON J.R., GOETZ E., GOETZ R., GONDAN L., GONZALEZ G., GONZALEZ CASTRO J.M., GOPAKUMAR A., GORDON N.A., GORODETSKY M.L., GOSSAN S.E., GOSSELIN M., GOUATY R., GRAEF C., GRAFF P.B., GRANATA M., GRANT A., GRAS S., GRAY C., GRECO G., GREEN A.C., GREENHALGH R.J.S., GROOT P., GROTE H., GRUNEWALD S., GUIDI G.M., GUO X., GUPTA A., GUPTA M.K., GUSHWA K.E., GUSTAFSON E.K., GUSTAFSON R., HACKER J.J., HALL B.R., HALL E.D., HAMMOND G., HANEY M., HANKE M.M., HANKS J., HANNA C., HANNAM M.D., HANSON J., HARDWICK T., HARMS J., HARRY G.M., HARRY I.W., HART M.J., HARTMAN M.T., HASTER C.-J., HAUGHIAN K., HEALY J., HEEFNER J., HEIDMANN A., HEINTZE M.C., HEINZEL G., HEITMANN H., HELLO P., HEMMING G., HENDRY M., HENG I.S., HENNIG J., HEPTONSTALL A.W., HEURS M., HILD S., HOAK D., HODGE K.A., HOFMAN D., HOLLITT S.E., HOLT K., HOLZ D.E., HOPKINS P., HOSKEN D.J., HOUGH J., HOUSTON E.A., HOWELL E.J., HU Y.M., HUANG S., HUERTA E.A., HUET D., HUGHEY B., HUSA S., HUTTNER S.H., HUYNH-DINH T., IDRISY A., INDIK N., INGRAM D.R., INTA R., ISA H.N., ISAC J.-M., ISI M., ISLAS G., ISOGAI T., IYER B.R., IZUMI K., JACOBSON M.B., JACQMIN T., JANG H., JANI K., JARANOWSKI P., JAWAHAR S., JIMENEZ-FORTEZA F., JOHNSON W.W., JOHNSON-McDANIEL N.K., JONES D.I., JONES R., JONKER R.J.G., JU L., HARIS K., KALAGHATGI C.V., KALOGERA V., KANDHASAMY S., KANG G., KANNER J.B., KARKI S., KASPRZACK M., KATSAVOUNIDIS E., KATZMAN W., KAUFER S., KAUR T., KAWABE K., KAWAZOE F., KEFELIAN F., KEHL M.S., KEITEL D., KELLEY D.B., KELLS W., KENNEDY R., KEPPEL D.G., KEY J.S., KHALAIDOVSKI A., KHALILI F.Y., KHAN I., KHAN S., KHAN Z., KHAZANOV E.A., KIJBUNCHOO N., KIM C., KIM J., KIM K., KIM N.-G., KIM N., KIM Y.-M., KING E.J., KING P.J., KINZEL D.L., KISSEL J.S., KLEYBOLTE L., KLIMENKO S., KOEHLENBECK S.M., KOKEYAMA K., KOLEY S., KONDRASHOV V., KONTOS A., KORANDA S., KOROBKO M., KORTH W.Z., KOWALSKA I., KOZAK D.B., KRINGEL V., KRISHNAN B., KROLAK A., KRUEGER C., KUEHN G., KUMAR P., KUMAR R., KUO L., KUTYNIA A., KWEE P., LACKEY B.D., LANDRY M., LANGE J., LANTZ B., LASKY P.D., LAZZARINI A., LAZZARO C., LEACI P., LEAVEY S., LEBIGOT E.O., LEE C.H., LEE H.K., LEE H.M., LEE K., LENON A., LEONARDI M., LEONG J.R., LEROY N., LETENDRE N., LEVIN Y., LEVINE B.M., LI T.G.F., LIBSON A., LITTENBERG T.B., LOCKERBIE N.A., LOGUE J., LOMBARDI A.L., LONDON L.T., LORD J.E., LORENZINI M., LORIETTE V., LORMAND M., LOSURDO G., LOUGH J.D., LOUSTO C.O., LOVELACE G., LUCK H., LUNDGREN A.P., LUO J., LYNCH R., MA Y., MACDONALD T., MACHENSCHALK B., MACINNIS M., MACLEOD D.M., MAGANA-SANDOVAL F., MAGEE R.M., MAGESWARAN M., MAJORANA E., MAKSIMOVIC I., MALVEZZI V., MAN N., MANDEL I., MANDIC V., MANGANO V., MANSELL G.L., MANSKE M., MANTOVANI M., MARCHESONI F., MARION F., MARKA S., MARKA Z., MARKOSYAN A.S., MAROS E., MARTELLI F., MARTELLINI L., MARTIN I.W., MARTIN R.M., MARTYNOV D.V., MARX J.N., MASON K., MASSEROT A., MASSINGER T.J., MASSO-REID M., MATICHARD F., MATONE L., MAVALVALA N., MAZUMDER N., MAZZOLO G., McCARTHY R., McCLELLAND D.E., McCORMICK S., McGUIRE S.C., McINTYRE G., McIVER J., McMANUS D.J., McWILLIAMS S.T., MEACHER D., MEADORS G.D., MEIDAM J., MELATOS A., MENDELL G., MENDOZA-GANDARA D., MERCER R.A., MERILH E., MERZOUGUI M., MESHKOV S., MESSENGER C., MESSICK C., MEYERS P.M., MEZZANI F., MIAO H., MICHEL C., MIDDLETON H., MIKHAILOV E.E., MILANO L., MILLER J., MILLHOUSE M., MINENKOV Y., MING J., MIRSHEKARI S., MISHRA C., MITRA S., MITROFANOV V.P., MITSELMAKHER G., MITTLEMAN R., MOGGI A., MOHAN M., MOHAPATRA S.R.P., MONTANI M., MOORE B.C., MOORE C.J., MORARU D., MORENO G., MORRISS S.R., MOSSAVI K., MOURS B., MOW-LOWRY C.M., MUELLER C.L., MUELLER G., MUIR A.W., MUKHERJEE A., MUKHERJEE D., MUKHERJEE S., MUKUND N., MULLAVEY A., MUNCH J., MURPHY D.J., MURRAY P.G., MYTIDIS A., NARDECCHIA I., NATICCHIONI L., NAYAK R.K., NECULA V., NEDKOVA K., NELEMANS G., NERI M., NEUNZERT A., NEWTON G., NGUYEN T.T., NIELSEN A.B., NISSANKE S., NITZ A., NOCERA F., NOLTING D., NORMANDIN M.E.N., NUTTALL L.K., OBERLING J., OCHSNER E., O'DELL J., OELKER E., OGIN G.H., OH J.J., OH S.H., OHME F., OLIVER M., OPPERMANN P., ORAM R.J., O'REILLY B., O'SHAUGHNESSY R., OTT C.D., OTTAWAY D.J., OTTENS R.S., OVERMIER H., OWEN B.J., PAI A., PAI S.A., PALAMOS J.R., PALASHOV O., PALOMBA C., PAL-SINGH A., PAN H., PAN Y., PANKOW C., PANNARALE F., PANT B.C., PAOLETTI F., PAOLI A., PAPA M.A., PARIS H.R., PARKER W., PASCUCCI D., PASQUALETTI A., PASSAQUIETI R., PASSUELLO D., PATRICELLI B., PATRICK Z., PEARLSTONE B.L., PEDRAZA M., PEDURAND R., PEKOWSKY L., PELE A., PENN S., PERRECA A., PFEIFFER H.P., PHELPS M., PICCINNI O., PICHOT M., PICKENPACK M., PIERGIOVANNI F., PIERRO V., PILLANT G., PINARD L., PINTO I.M., PITKIN M., POELD J.H., POGGIANI R., POPOLIZIO P., POST A., POWELL J., PRASAD J., PREDOI V., PREMACHANDRA S.S., PRESTEGARD T., PRICE L.R., PRIJATELJ M., PRINCIPE M., PRIVITERA S., PRIX R., PRODI G.A., PROKHOROV L., PUNCKEN O., PUNTURO M., PUPPO P., PURRER M., QI H., QIN J., QUETSCHKE V., QUINTERO E.A., QUITZOW-JAMES R., RAAB F.J., RABELING D.S., RADKINS H., RAFFAI P., RAJA S., RAKHMANOV M., RAMET C.R., RAPAGNANI P., RAYMOND V., RAZZANO M., RE V., READ J., REED C.M., REGIMBAU T., REI L., REID S., REITZE D.H., REW H., REYES S.D., RICCI F., RILES K., ROBERTSON N.A., ROBIE R., ROBINET F., ROCCHI A., ROLLAND L., ROLLINS J.G., ROMA V.J., ROMANO J.D., ROMANO R., ROMANOV G., ROMIE J.H., ROSINSKA D., ROWAN S., RUDIGER A., RUGGI P., RYAN K., SACHDEV S., SADECKI T., SADEGHIAN L., SALCONI L., SALEEM M., SALEMI F., SAMAJDAR A., SAMMUT L., SAMPSON L.M., SANCHEZ E.J., SANDBERG V., SANDEEN B., SANDERS G.H., SANDERS J.R., SASSOLAS B., SATHYAPRAKASH B.S., SAULSON P.R., SAUTER O., SAVAGE R.L., SAWADSKY A., SCHALE P., SCHILLING R., SCHMIDT J., SCHMIDT P., SCHNABEL R., SCHOFIELD R.M.S., SCHONBECK A., SCHREIBER E., SCHUETTE D., SCHUTZ B.F., SCOTT J., SCOTT S.M., SELLERS D., SENGUPTA A.S., SENTENAC D., SEQUINO V., SERGEEV A., SERNA G., SETYAWATI Y., SEVIGNY A., SHADDOCK D.A., SHAFFER T., SHAH S., SHAHRIAR M.S., SHALTEV M., SHAO Z., SHAPIRO B., SHAWHAN P., SHEPERD A., SHOEMAKER D.H., SHOEMAKER D.M., SIELLEZ K., SIEMENS X., SIGG D., SILVA A.D., SIMAKOV D., SINGER A., SINGER L.P., SINGH A., SINGH R., SINGHAL A., SINTES A.M., SLAGMOLEN B.J.J., SMITH J.R., SMITH M.R., SMITH N.D., SMITH R.J.E., SON E.J., SORAZU B., SORRENTINO F., SOURADEEP T., SRIVASTAVA A.K., STALEY A., STEINKE M., STEINLECHNER J., STEINLECHNER S., STEINMEYER D., STEPHENS B.C., STEVENSON S.P., STONE R., STRAIN K.A., STRANIERO N., STRATTA G., STRAUSS N.A., STRIGIN S., STURANI R., STUVER A.L., SUMMERSCALES T.Z., SUN L., SUTTON P.J., SWINKELS B.L., SZCZEPANCZYK M.J., TACCA M., TALUKDER D., TANNER D.B., TAPAI M., TARABRIN S.P., TARACCHINI A., TAYLOR R., THEEG T., THIRUGNANASAMBANDAM M.P., THOMAS E.G., THOMAS M., THOMAS P., THORNE K.A., THORNE K.S., THRANE E., TIWARI S., TIWARI V., TOKMAKOV K.V., TOMLINSON C., TONELLI M., TORRES C.V., TORRIE C.I., TOYRA D., TRAVASSO F., TRAYLOR G., TRIFIRO D., TRINGALI M.C., TROZZO L., TSE M., TURCONI M., TUYENBAYEV D., UGOLINI D., UNNIKRISHNAN C.S., URBAN A.L., USMAN S.A., VAHLBRUCH H., VAJENTE G., VALDES G., VALLISNERI M., VAN BAKEL N., VAN BEUZEKOM M., VAN DEN BRAND J.F.J., VAN DEN BROECK C., VANDER-HYDE D.C., VAN DER SCHAAF L., VAN HEIJNINGEN J.V., VAN VEGGEL A.A., VARDARO M., VASS S., VASUTH M., VAULIN R., VECCHIO A., VEDOVATO G., VEITCH J., VEITCH P.J., VENKATESWARA K., VERKINDT D., VETRANO F., VICERE A., VINCIGUERRA S., VINE D.J., VINET J.-Y., VITALE S., VO T., VOCCA H., VORVICK C., VOSS D., VOUSDEN W.D., VYATCHANIN S.P., WADE A.R., WADE L.E., WADE M., WALDMAN S.J., WALKER M., WALLACE L., WALSH S., WANG G., WANG H., WANG M., WANG X., WANG Y., WARD H., WARD R.L., WARNER J., WAS M., WEAVER B., WEI L.-W., WEINERT M., WEINSTEIN A.J., WEISS R., WELBORN T., WEN L., WESSELS P., WESTPHAL T., WETTE K., WHELAN J.T., WHITCOMB S.E., WHITE D.J., WHITING B.F., WIESNER K., WILKINSON C., WILLEMS P.A., WILLIAMS L., WILLIAMS R.D., WILLIAMSON A.R., WILLIS J.L., WILLKE B., WIMMER M.H., WINKELMANN L., WINKLER W., WIPF C.C., WISEMAN A.G., WITTEL H., WOAN G., WORDEN J., WRIGHT J.L., WU G., YABLON J., YAKUSHIN I., YAM W., YAMAMOTO H., YANCEY C.C., YAP M.J., YU H., YVERT M., ZADROZNY A., ZANGRANDO L., ZANOLIN M., ZENDRI J.-P., ZEVIN M., ZHANG F., ZHANG L., ZHANG M., ZHANG Y., ZHAO C., ZHOU M., ZHOU Z., ZHU X.J., ZUCKER M.E., ZURAW S.E., ZWEIZIG J., (The LIGO Scientific Collaboration), (The Virgo Collaboration)
	PhRvL, 116f, 1102 (2016)
	Observation of gravitational waves from a binary black hole merger.
o	<GrW YYMMDD> (No. 150914).
Ref:	=2016PhRvL.116x1103A
by	ABBOTT B.P. , ABBOTT R., ABBOTT T.D., ABERNATHY M.R., ACERNESE F., ACKLEY K., ADAMS C., ADAMS T., ADDESSO P., ADHIKARI R.X., ADYA V.B., AFFELDT C., AGATHOS M., AGATSUMA K., AGGARWAL N., AGUIAR O.D., AIELLO L., AIN A., AJITH P., ALLEN B., ALLOCCA A., ALTIN P.A., ANDERSON S.B., ANDERSON W.G., ARAI K., ARAIN M.A., ARAYA M.C., ARCENEAUX C.C., AREEDA J.S., ARNAUD N., ARUN K.G., ASCENZI S., ASHTON G., AST M., ASTON S.M., ASTONE P., AUFMUTH P., AULBERT C., BABAK S., BACON P., BADER M.K.M., BAKER P.T., BALDACCINI F., BALLARDIN G., BALLMER S.W., BARAYOGA J.C., BARCLAY S.E., BARISH B.C., BARKER D., BARONE F., BARR B., BARSOTTI L., BARSUGLIA M., BARTA D., BARTLETT J., BARTON M.A., BARTOS I., BASSIRI R., BASTI A., BATCH J.C., BAUNE C., BAVIGADDA V., BAZZAN M., BEHNKE B., BEJGER M., BELCZYNSKI C., BELL A.S., BELL C.J., BERGER B.K., BERGMAN J., BERGMANN G., BERRY C.P.L., BERSANETTI D., BERTOLINI A., BETZWIESER J., BHAGWAT S., BHANDARE R., BILENKO I.A., BILLINGSLEY G., BIRCH J., BIRNEY R., BIRNHOLTZ O., BISCANS S., BISHT A., BITOSSI M., BIWER C., BIZOUARD M.A., BLACKBURN J.K., BLAIR C.D., BLAIR D.G., BLAIR R.M., BLOEMEN S., BOCK O., BODIYA T.P., BOER M., BOGAERT G., BOGAN C., BOHE A., BOJTOS P., BOND C., BONDU F., BONNAND R., BOOM B.A., BORK R., BOSCHI V., BOSE S., BOUFFANAIS Y., BOZZI A., BRADASCHIA C., BRADY P.R., BRAGINSKY V.B., BRANCHESI M., BRAU J.E., BRIANT T., BRILLET A., BRINKMANN M., BRISSON V., BROCKILL P., BROOKS A.F., BROWN D.A., BROWN D.D., BROWN N.M., BUCHANAN C.C., BUIKEMA A., BULIK T., BULTEN H.J., BUONANNO A., BUSKULIC D., BUY C., BYER R.L., CABERO M., CADONATI L., CAGNOLI G., CAHILLANE C., CALDERON BUSTILLO J., CALLISTER T., CALLONI E., CAMP J.B., CANNON K.C., CAO J., CAPANO C.D., CAPOCASA E., CARBOGNANI F., CARIDE S., CASANUEVA DIAZ J., CASENTINI C., CAUDILL S., CAVAGLIA M., CAVALIER F., CAVALIERI R., CELLA G., CEPEDA C.B., CERBONI BAIARDI L., CERRETANI G., CESARINI E., CHAKRABORTY R., CHALERMSONGSAK T., CHAMBERLIN S.J., CHAN M., CHAO S., CHARLTON P., CHASSANDE-MOTTIN E., CHEN H.Y., CHEN Y., CHENG C., CHINCARINI A., CHIUMMO A., CHO H.S., CHO M., CHOW J.H., CHRISTENSEN N., CHU Q., CHUA S., CHUNG S., CIANI G., CLARA F., CLARK J.A., CLEVA F., COCCIA E., COHADON P.-F., COLLA A., COLLETTE C.G., COMINSKY L., CONSTANCIO M., CONTE A., CONTI L., COOK D., CORBITT T.R., CORNISH N., CORSI A., CORTESE S., COSTA C.A., COUGHLIN M.W., COUGHLIN S.B., COULON J.-P., COUNTRYMAN S.T., COUVARES P., COWAN E.E., COWARD D.M., COWART M.J., COYNE D.C., COYNE R., CRAIG K., CREIGHTON J.D.E., CREIGHTON T.D., CRIPE J., CROWDER S.G., CRUISE A.M., CUMMING A., CUNNINGHAM L., CUOCO E., DAL CANTON T., DANILISHIN S.L., D'ANTONIO S., DANZMANN K., DARMAN N.S., DA SILVA COSTA C.F., DATTILO V., DAVE I., DAVELOZA H.P., DAVIER M., DAVIES G.S., DAW E.J., DAY R., DE S., DEBRA D., DEBRECZENI G., DEGALLAIX J., DE LAURENTIS M., DELEGLISE S., DEL POZZO W., DENKER T., DENT T., DERELI H., DERGACHEV V., DEROSA R.T., DE ROSA R., DESALVO R., DHURANDHAR S., DIAZ M.C., DI FIORE L., DI GIOVANNI M., DI LIETO A., DI PACE S., DI PALMA I., DI VIRGILIO A., DOJCINOSKI G., DOLIQUE V., DONOVAN F., DOOLEY K.L., DORAVARI S., DOUGLAS R., DOWNES T.P., DRAGO M., DREVER R.W.P., DRIGGERS J.C., DU Z., DUCROT M., DWYER S.E., EDO T.B., EDWARDS M.C., EFFLER A., EGGENSTEIN H.-B., EHRENS P., EICHHOLZ J., EIKENBERRY S.S., ENGELS W., ESSICK R.C., ETZEL T., EVANS M., EVANS T.M., EVERETT R., FACTOUROVICH M., FAFONE V., FAIR H., FAIRHURST S., FAN X., FANG Q., FARINON S., FARR B., FARR W.M., FAVATA M., FAYS M., FEHRMANN H., FEJER M.M., FELDBAUM D., FERRANTE I., FERREIRA E.C., FERRINI F., FIDECARO F., FINN L.S., FIORI I., FIORUCCI D., FISHER R.P., FLAMINIO R., FLETCHER M., FONG H., FOURNIER J.-D., FRANCO S., FRASCA S., FRASCONI F., FREDE M., FREI Z., FREISE A., FREY R., FREY V., FRICKE T.T., FRITSCHEL P., FROLOV V.V., FULDA P., FYFFE M., GABBARD H.A.G., GAIR J.R., GAMMAITONI L., GAONKAR S.G., GARUFI F., GATTO A., GAUR G., GEHRELS N., GEMME G., GENDRE B., GENIN E., GENNAI A., GEORGE J., GERGELY L., GERMAIN V., GHOSH A., GHOSH A., GHOSH S., GIAIME J.A., GIARDINA K.D., GIAZOTTO A., GILL K., GLAEFKE A., GLEASON J.R., GOETZ E., GOETZ R., GONDAN L., GONZALEZ G., GONZALEZ CASTRO J.M., GOPAKUMAR A., GORDON N.A., GORODETSKY M.L., GOSSAN S.E., GOSSELIN M., GOUATY R., GRAEF C., GRAFF P.B., GRANATA M., GRANT A., GRAS S., GRAY C., GRECO G., GREEN A.C., GREENHALGH R.J.S., GROOT P., GROTE H., GRUNEWALD S., GUIDI G.M., GUO X., GUPTA A., GUPTA M.K., GUSHWA K.E., GUSTAFSON E.K., GUSTAFSON R., HACKER J.J., HALL B.R., HALL E.D., HAMMOND G., HANEY M., HANKE M.M., HANKS J., HANNA C., HANNAM M.D., HANSON J., HARDWICK T., HARMS J., HARRY G.M., HARRY I.W., HART M.J., HARTMAN M.T., HASTER C.-J., HAUGHIAN K., HEALY J., HEEFNER J., HEIDMANN A., HEINTZE M.C., HEINZEL G., HEITMANN H., HELLO P., HEMMING G., HENDRY M., HENG I.S., HENNIG J., HEPTONSTALL A.W., HEURS M., HILD S., HOAK D., HODGE K.A., HOFMAN D., HOLLITT S.E., HOLT K., HOLZ D.E., HOPKINS P., HOSKEN D.J., HOUGH J., HOUSTON E.A., HOWELL E.J., HU Y.M., HUANG S., HUERTA E.A., HUET D., HUGHEY B., HUSA S., HUTTNER S.H., HUYNH-DINH T., IDRISY A., INDIK N., INGRAM D.R., INTA R., ISA H.N., ISAC J.-M., ISI M., ISLAS G., ISOGAI T., IYER B.R., IZUMI K., JACOBSON M.B., JACQMIN T., JANG H., JANI K., JARANOWSKI P., JAWAHAR S., JIMENEZ-FORTEZA F., JOHNSON W.W., JOHNSON-McDANIEL N.K., JONES D.I., JONES R., JONKER R.J.G., JU L., HARIS K., KALAGHATGI C.V., KALOGERA V., KANDHASAMY S., KANG G., KANNER J.B., KARKI S., KASPRZACK M., KATSAVOUNIDIS E., KATZMAN W., KAUFER S., KAUR T., KAWABE K., KAWAZOE F., KEFELIAN F., KEHL M.S., KEITEL D., KELLEY D.B., KELLS W., KENNEDY R., KEPPEL D.G., KEY J.S., KHALAIDOVSKI A., KHALILI F.Y., KHAN I., KHAN S., KHAN Z., KHAZANOV E.A., KIJBUNCHOO N., KIM C., KIM J., KIM K., KIM N.-G., KIM N., KIM Y.-M., KING E.J., KING P.J., KINZEL D.L., KISSEL J.S., KLEYBOLTE L., KLIMENKO S., KOEHLENBECK S.M., KOKEYAMA K., KOLEY S., KONDRASHOV V., KONTOS A., KORANDA S., KOROBKO M., KORTH W.Z., KOWALSKA I., KOZAK D.B., KRINGEL V., KRISHNAN B., KROLAK A., KRUEGER C., KUEHN G., KUMAR P., KUMAR R., KUO L., KUTYNIA A., KWEE P., LACKEY B.D., LANDRY M., LANGE J., LANTZ B., LASKY P.D., LAZZARINI A., LAZZARO C., LEACI P., LEAVEY S., LEBIGOT E.O., LEE C.H., LEE H.K., LEE H.M., LEE K., LENON A., LEONARDI M., LEONG J.R., LEROY N., LETENDRE N., LEVIN Y., LEVINE B.M., LI T.G.F., LIBSON A., LITTENBERG T.B., LOCKERBIE N.A., LOGUE J., LOMBARDI A.L., LONDON L.T., LORD J.E., LORENZINI M., LORIETTE V., LORMAND M., LOSURDO G., LOUGH J.D., LOUSTO C.O., LOVELACE G., LUCK H., LUNDGREN A.P., LUO J., LYNCH R., MA Y., MACDONALD T., MACHENSCHALK B., MACINNIS M., MACLEOD D.M., MAGANA-SANDOVAL F., MAGEE R.M., MAGESWARAN M., MAJORANA E., MAKSIMOVIC I., MALVEZZI V., MAN N., MANDEL I., MANDIC V., MANGANO V., MANSELL G.L., MANSKE M., MANTOVANI M., MARCHESONI F., MARION F., MARKA S., MARKA Z., MARKOSYAN A.S., MAROS E., MARTELLI F., MARTELLINI L., MARTIN I.W., MARTIN R.M., MARTYNOV D.V., MARX J.N., MASON K., MASSEROT A., MASSINGER T.J., MASSO-REID M., MATICHARD F., MATONE L., MAVALVALA N., MAZUMDER N., MAZZOLO G., McCARTHY R., McCLELLAND D.E., McCORMICK S., McGUIRE S.C., McINTYRE G., McIVER J., McMANUS D.J., McWILLIAMS S.T., MEACHER D., MEADORS G.D., MEIDAM J., MELATOS A., MENDELL G., MENDOZA-GANDARA D., MERCER R.A., MERILH E., MERZOUGUI M., MESHKOV S., MESSENGER C., MESSICK C., MEYERS P.M., MEZZANI F., MIAO H., MICHEL C., MIDDLETON H., MIKHAILOV E.E., MILANO L., MILLER J., MILLHOUSE M., MINENKOV Y., MING J., MIRSHEKARI S., MISHRA C., MITRA S., MITROFANOV V.P., MITSELMAKHER G., MITTLEMAN R., MOGGI A., MOHAN M., MOHAPATRA S.R.P., MONTANI M., MOORE B.C., MOORE C.J., MORARU D., MORENO G., MORRISS S.R., MOSSAVI K., MOURS B., MOW-LOWRY C.M., MUELLER C.L., MUELLER G., MUIR A.W., MUKHERJEE A., MUKHERJEE D., MUKHERJEE S., MUKUND N., MULLAVEY A., MUNCH J., MURPHY D.J., MURRAY P.G., MYTIDIS A., NARDECCHIA I., NATICCHIONI L., NAYAK R.K., NECULA V., NEDKOVA K., NELEMANS G., NERI M., NEUNZERT A., NEWTON G., NGUYEN T.T., NIELSEN A.B., NISSANKE S., NITZ A., NOCERA F., NOLTING D., NORMANDIN M.E.N., NUTTALL L.K., OBERLING J., OCHSNER E., O'DELL J., OELKER E., OGIN G.H., OH J.J., OH S.H., OHME F., OLIVER M., OPPERMANN P., ORAM R.J., O'REILLY B., O'SHAUGHNESSY R., OTT C.D., OTTAWAY D.J., OTTENS R.S., OVERMIER H., OWEN B.J., PAI A., PAI S.A., PALAMOS J.R., PALASHOV O., PALOMBA C., PAL-SINGH A., PAN H., PAN Y., PANKOW C., PANNARALE F., PANT B.C., PAOLETTI F., PAOLI A., PAPA M.A., PARIS H.R., PARKER W., PASCUCCI D., PASQUALETTI A., PASSAQUIETI R., PASSUELLO D., PATRICELLI B., PATRICK Z., PEARLSTONE B.L., PEDRAZA M., PEDURAND R., PEKOWSKY L., PELE A., PENN S., PERRECA A., PFEIFFER H.P., PHELPS M., PICCINNI O., PICHOT M., PICKENPACK M., PIERGIOVANNI F., PIERRO V., PILLANT G., PINARD L., PINTO I.M., PITKIN M., POELD J.H., POGGIANI R., POPOLIZIO P., POST A., POWELL J., PRASAD J., PREDOI V., PREMACHANDRA S.S., PRESTEGARD T., PRICE L.R., PRIJATELJ M., PRINCIPE M., PRIVITERA S., PRIX R., PRODI G.A., PROKHOROV L., PUNCKEN O., PUNTURO M., PUPPO P., PURRER M., QI H., QIN J., QUETSCHKE V., QUINTERO E.A., QUITZOW-JAMES R., RAAB F.J., RABELING D.S., RADKINS H., RAFFAI P., RAJA S., RAKHMANOV M., RAMET C.R., RAPAGNANI P., RAYMOND V., RAZZANO M., RE V., READ J., REED C.M., REGIMBAU T., REI L., REID S., REITZE D.H., REW H., REYES S.D., RICCI F., RILES K., ROBERTSON N.A., ROBIE R., ROBINET F., ROCCHI A., ROLLAND L., ROLLINS J.G., ROMA V.J., ROMANO J.D., ROMANO R., ROMANOV G., ROMIE J.H., ROSINSKA D., ROWAN S., RUDIGER A., RUGGI P., RYAN K., SACHDEV S., SADECKI T., SADEGHIAN L., SALCONI L., SALEEM M., SALEMI F., SAMAJDAR A., SAMMUT L., SAMPSON L.M., SANCHEZ E.J., SANDBERG V., SANDEEN B., SANDERS G.H., SANDERS J.R., SASSOLAS B., SATHYAPRAKASH B.S., SAULSON P.R., SAUTER O., SAVAGE R.L., SAWADSKY A., SCHALE P., SCHILLING R., SCHMIDT J., SCHMIDT P., SCHNABEL R., SCHOFIELD R.M.S., SCHONBECK A., SCHREIBER E., SCHUETTE D., SCHUTZ B.F., SCOTT J., SCOTT S.M., SELLERS D., SENGUPTA A.S., SENTENAC D., SEQUINO V., SERGEEV A., SERNA G., SETYAWATI Y., SEVIGNY A., SHADDOCK D.A., SHAFFER T., SHAH S., SHAHRIAR M.S., SHALTEV M., SHAO Z., SHAPIRO B., SHAWHAN P., SHEPERD A., SHOEMAKER D.H., SHOEMAKER D.M., SIELLEZ K., SIEMENS X., SIGG D., SILVA A.D., SIMAKOV D., SINGER A., SINGER L.P., SINGH A., SINGH R., SINGHAL A., SINTES A.M., SLAGMOLEN B.J.J., SMITH J.R., SMITH M.R., SMITH N.D., SMITH R.J.E., SON E.J., SORAZU B., SORRENTINO F., SOURADEEP T., SRIVASTAVA A.K., STALEY A., STEINKE M., STEINLECHNER J., STEINLECHNER S., STEINMEYER D., STEPHENS B.C., STEVENSON S.P., STONE R., STRAIN K.A., STRANIERO N., STRATTA G., STRAUSS N.A., STRIGIN S., STURANI R., STUVER A.L., SUMMERSCALES T.Z., SUN L., SUTTON P.J., SWINKELS B.L., SZCZEPANCZYK M.J., TACCA M., TALUKDER D., TANNER D.B., TAPAI M., TARABRIN S.P., TARACCHINI A., TAYLOR R., THEEG T., THIRUGNANASAMBANDAM M.P., THOMAS E.G., THOMAS M., THOMAS P., THORNE K.A., THORNE K.S., THRANE E., TIWARI S., TIWARI V., TOKMAKOV K.V., TOMLINSON C., TONELLI M., TORRES C.V., TORRIE C.I., TOYRA D., TRAVASSO F., TRAYLOR G., TRIFIRO D., TRINGALI M.C., TROZZO L., TSE M., TURCONI M., TUYENBAYEV D., UGOLINI D., UNNIKRISHNAN C.S., URBAN A.L., USMAN S.A., VAHLBRUCH H., VAJENTE G., VALDES G., VALLISNERI M., VAN BAKEL N., VAN BEUZEKOM M., VAN DEN BRAND J.F.J., VAN DEN BROECK C., VANDER-HYDE D.C., VAN DER SCHAAF L., VAN HEIJNINGEN J.V., VAN VEGGEL A.A., VARDARO M., VASS S., VASUTH M., VAULIN R., VECCHIO A., VEDOVATO G., VEITCH J., VEITCH P.J., VENKATESWARA K., VERKINDT D., VETRANO F., VICERE A., VINCIGUERRA S., VINE D.J., VINET J.-Y., VITALE S., VO T., VOCCA H., VORVICK C., VOSS D., VOUSDEN W.D., VYATCHANIN S.P., WADE A.R., WADE L.E., WADE M., WALDMAN S.J., WALKER M., WALLACE L., WALSH S., WANG G., WANG H., WANG M., WANG X., WANG Y., WARD H., WARD R.L., WARNER J., WAS M., WEAVER B., WEI L.-W., WEINERT M., WEINSTEIN A.J., WEISS R., WELBORN T., WEN L., WESSELS P., WESTPHAL T., WETTE K., WHELAN J.T., WHITCOMB S.E., WHITE D.J., WHITING B.F., WIESNER K., WILKINSON C., WILLEMS P.A., 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	PhRvL, 116x, 1103 (2016)
	GW151226: observation of gravitational waves from a 22-solar-mass binary black hole coalescence.
o	<GrW YYMMDD> (No. 151226).
Ref:	=2017PhRvL.118v1101A
by	ABBOTT B.P. , ABBOTT R., ABBOTT T.D., ACERNESE F., ACKLEY K., ADAMS C., ADAMS T., ADDESSO P., ADHIKARI R.X., ADYA V.B., AFFELDT C., AFROUGH M., AGARWAL B., AGATHOS M., AGATSUMA K., AGGARWAL N., AGUIAR O.D., AIELLO L., AIN A., AJITH P., ALLEN B., ALLEN G., ALLOCCA A., ALTIN P.A., AMATO A., ANANYEVA A., ANDERSON S.B., ANDERSON W.G., ANTIER S., APPERT S., ARAI K., ARAYA M.C., AREEDA J.S., ARNAUD N., ARUN K.G., ASCENZI S., ASHTON G., AST M., ASTON S.M., ASTONE P., AUFMUTH P., AULBERT C., NEAL K., AVILA-ALVAREZ A., BABAK S., BACON P., BADER M.K.M., BAE S., BAKER P.T., BALDACCINI F., BALLARDIN G., BALLMER S.W., BANAGIRI S., BARAYOGA J.C., BARCLAY S.E., BARISH B.C., BARKER D., BARONE F., BARR B., BARSOTTI L., BARSUGLIA M., BARTA D., BARTLETT J., BARTOS I., BASSIRI R., BASTI A., BATCH J.C., BAUNE C., BAWAJ M., BAZZAN M., BECSY B., BEER C., BEJGER M., BELAHCENE I., BELL A.S., BERGER B.K., BERGMANN G., BERRY C.P.L., BERSANETTI D., BERTOLINI A., BETZWIESER J., BHAGWAT S., BHANDARE R., BILENKO I.A., BILLINGSLEY G., BILLMAN C.R., BIRCH J., BIRNEY R., BIRNHOLTZ O., BISCANS S., BISHT A., BITOSSI M., BIWER C., BIZOUARD M.A., BLACKBURN J.K., BLACKMAN J., BLAIR C.D., BLAIR D.G., BLAIR R.M., BLOEMEN S., BOCK O., BODE N., BOER M., BOGAERT G., BOHE A., BONDU F., BONNAND R., BOOM B.A., BORK R., BOSCHI V., BOSE S., BOUFFANAIS Y., BOZZI A., BRADASCHIA C., BRADY P.R., BRAGINSKY V.B., BRANCHESI M., BRAU J.E., BRIANT T., BRILLET A., BRINKMANN M., BRISSON V., BROCKILL P., BROIDA J.E., BROOKS A.F., BROWN D.A., BROWN D.D., BROWN N.M., BRUNETT S., BUCHANAN C.C., BUIKEMA A., BULIK T., BULTEN H.J., BUONANNO A., BUSKULIC D., BUY C., BYER R.L., CABERO M., CADONATI L., CAGNOLI G., CAHILLANE C., CALDERON BUSTILLO J., CALLISTER T.A., CALLONI E., CAMP J.B., CANEPA M., CANIZARES P., CANNON K.C., CAO H., CAO J., CAPANO C.D., CAPOCASA E., CARBOGNANI F., CARIDE S., CARNEY M.F., CASANUEVA DIAZ J., CASENTINI C., CAUDILL S., CAVAGLIA M., CAVALIER F., CAVALIERI R., CELLA G., CEPEDA C.B., CERBONI BAIARDI L., CERRETANI G., CESARINI E., CHAMBERLIN S.J., CHAN M., CHAO S., CHARLTON P., CHASSANDE-MOTTIN E., CHATTERJEE D., CHATZIIOANNOU K., CHEESEBORO B.D., CHEN H.Y., CHEN Y., CHENG H., CHINCARINI A., CHIUMMO A., CHMIEL T., CHO H.S., CHO M., CHOW J.H., CHRISTENSEN N., CHU Q., CHUA A.J.K., CHUA S., CHUNG A.K.W., CHUNG S., CIANI G., CIOLFI R., CIRELLI C.E., CIRONE A., CLARA F., CLARK J.A., CLEVA F., COCCHIERI C., COCCIA E., COHADON P., COLLA A., COLLETTE C.G., COMINSKY L.R., CONSTANCIO M., CONTI L., COOPER S.J., CORBAN P., CORBITT T.R., CORLEY K.R., CORNISH N., CORSI A., CORTESE S., COSTA C.A., COUGHLIN M.W., COUGHLIN S.B., COULON J., COUNTRYMAN S.T., COUVARES P., COVAS P.B., COWAN E.E., COWARD D.M., COWART M.J., COYNE D.C., COYNE R., CREIGHTON J.D.E., CREIGHTON T.D., CRIPE J., CROWDER S.G., CULLEN T.J., CUMMING A., CUNNINGHAM L., CUOCO E., DAL CANTON T., DANILISHIN S.L., D'ANTONIO S., DANZMANN K., DASGUPTA A., SILVA COSTA C.F., DATTILO V., DAVE I., DAVIER M., DAVIS D., DAW E.J., DAY B., DE S., DEBRA D., DEELMAN E., DEGALLAIX J., DE LAURENTIS M., DELEGLISE S., DEL POZZO W., DENKER T., DENT T., DERGACHEV V., DE ROSA R., DEROSA R.T., DESALVO R., DEVENSON J., DEVINE R.C., DHURANDHAR S., DIAZ M.C., DI FIORE L., DI GIOVANNI M., DI GIROLAMO T., DI LIETO A., DI PACE S., DI PALMA I., DI RENZO F., DOCTOR Z., DOLIQUE V., DONOVAN F., DOOLEY K.L., DORAVARI S., DORRINGTON I., DOUGLAS R., DOVALE ALVAREZ M., DOWNES T.P., DRAGO M., DREVER R.W.P., DRIGGERS J.C., DU Z., DUCROT M., DUNCAN J., DWYER S.E., EDO T.B., EDWARDS M.C., EFFLER A., EGGENSTEIN H., EHRENS P., EICHHOLZ J., EIKENBERRY S.S., EISENSTEIN R.A., ESSICK R.C., ETIENNE Z.B., ETZEL T., EVANS M., EVANS T.M., FACTOUROVICH M., FAFONE V., FAIR H., FAIRHURST S., FAN X., FARINON S., FARR B., FARR W.M., FAUCHON-JONES E.J., FAVATA M., FAYS M., FEHRMANN H., FEICHT J., FEJER M.M., FERNANDEZ-GALIANA A., FERRANTE I., FERREIRA E.C., FERRINI F., FIDECARO F., FIORI I., FIORUCCI D., FISHER R.P., FLAMINIO R., FLETCHER M., FONG H., FORSYTH P.W.F., FORSYTH S.S., FOURNIER J., FRASCA S., FRASCONI F., FREI Z., FREISE A., FREY R., FREY V., FRIES E.M., FRITSCHEL P., FROLOV V.V., FULDA P., FYFFE M., GABBARD H., GABEL M., GADRE B.U., GAEBEL S.M., GAIR J.R., GAMMAITONI L., GANIJA M.R., GAONKAR S.G., GARUFI F., GAUDIO S., GAUR G., GAYATHRI V., GEHRELS N., GEMME G., GENIN E., GENNAI A., GEORGE D., GEORGE J., GERGELY L., GERMAIN V., GHONGE S., GHOSH A., GHOSH S., GIAIME J.A., GIARDINA K.D., GIAZOTTO A., GILL K., GLOVER L., GOETZ E., GOETZ R., GOMES S., GONZALEZ G., GONZALEZ CASTRO J.M., GOPAKUMAR A., GORODETSKY M.L., GOSSAN S.E., GOSSELIN M., GOUATY R., GRADO A., GRAEF C., GRANATA M., GRANT A., GRAS S., GRAY C., GRECO G., GREEN A.C., GROOT P., GROTE H., GRUNEWALD S., GRUNING P., GUIDI G.M., GUO X., GUPTA A., GUPTA M.K., GUSHWA K.E., GUSTAFSON E.K., GUSTAFSON R., HALL B.R., HALL E.D., HAMMOND G., HANEY M., HANKE M.M., HANKS J., HANNA C., HANNAM M.D., HANNUKSELA O.A., HANSON J., HARDWICK T., HARMS J., HARRY G.M., HARRY I.W., HART M.J., HASTER C., HAUGHIAN K., HEALY J., HEIDMANN A., HEINTZE M.C., HEITMANN H., HELLO P., HEMMING G., HENDRY M., HENG I.S., HENNIG J., HENRY J., HEPTONSTALL A.W., HEURS M., HILD S., HOAK D., HOFMAN D., HOLT K., HOLZ D.E., HOPKINS P., HORST C., HOUGH J., HOUSTON E.A., HOWELL E.J., HU Y.M., HUERTA E.A., HUET D., HUGHEY B., HUSA S., HUTTNER S.H., HUYNH-DINH T., INDIK N., INGRAM D.R., INTA R., INTINI G., ISA H.N., ISAC J., ISI M., IYER B.R., IZUMI K., JACQMIN T., JANI K., JARANOWSKI P., JAWAHAR S., JIMENEZ-FORTEZA F., JOHNSON W.W., McDANIEL N.K., JONES D.I., JONES R., JONKER R.J.G., JU L., JUNKER J., KALAGHATGI C.V., KALOGERA V., KANDHASAMY S., KANG G., KANNER J.B., KARKI S., KARVINEN K.S., KASPRZACK M., KATOLIK M., KATSAVOUNIDIS E., KATZMAN W., KAUFER S., KAWABE K., KEFELIAN F., KEITEL D., KEMBALL A.J., KENNEDY R., KENT C., KEY J.S., KHALILI F.Y., KHAN I., KHAN S., KHAN Z., KHAZANOV E.A., KIJBUNCHOO N., KIM C., KIM J.C., KIM W., KIM W.S., KIM Y., KIMBRELL S.J., KING E.J., KING P.J., KIRCHHOFF R., KISSEL J.S., KLEYBOLTE L., KLIMENKO S., KOCH P., KOEHLENBECK S.M., KOLEY S., KONDRASHOV V., KONTOS A., KOROBKO M., KORTH W.Z., KOWALSKA I., KOZAK D.B., KRAMER C., KRINGEL V., KRISHNAN B., KROLAK A., KUEHN G., KUMAR P., KUMAR R., KUMAR S., KUO L., KUTYNIA A., KWANG S., LACKEY B.D., LAI K.H., LANDRY M., LANG R.N., LANGE J., LANTZ B., LANZA R.K., LARTAUX-VOLLARD A., LASKY P.D., LAXEN M., LAZZARINI A., LAZZARO C., LEACI P., LEAVEY S., LEE C.H., LEE H.K., LEE H.M., LEE H.W., LEE K., LEHMANN J., LENON A., LEONARDI M., LEROY N., LETENDRE N., LEVIN Y., LI T.G.F., LIBSON A., LITTENBERG T.B., LIU J., LO R.K.L., LOCKERBIE N.A., LONDON L.T., LORD J.E., LORENZINI M., LORIETTE V., LORMAND M., LOSURDO G., LOUGH J.D., LOVELACE G., LUCK H., LUMACA D., LUNDGREN A.P., LYNCH R., MA Y., MacFOY S., MACHENSCHALK B., MACINNIS M., MacLEOD D.M., MAGANA HERNANDEZ I., MAGANA-SANDOVAL F., MAGANA ZERTUCHE L., MAGEE R.M., MAJORANA E., MAKSIMOVIC I., MAN N., MANDIC V., MANGANO V., MANSELL G.L., MANSKE M., MANTOVANI M., MARCHESONI F., MARION F., MARKA S., MARKA Z., MARKAKIS C., MARKOSYAN A.S., MAROS E., MARTELLI F., MARTELLINI L., MARTIN I.W., MARTYNOV D.V., MARX J.N., MASON K., MASSEROT A., MASSINGER T.J., MASSO-REID M., MASTROGIOVANNI S., MATAS A., MATICHARD F., MATONE L., MAVALVALA N., MAYANI R., MAZUMDER N., McCARTHY R., McCLELLAND D.E., McCORMICK S., McCULLER L., McGUIRE S.C., McINTYRE G., McIVER J., McMANUS D.J., McRAE T., McWILLIAMS S.T., MEACHER D., MEADORS G.D., MEIDAM J., MEJUTO-VILLA E., MELATOS A., MENDELL G., MERCER R.A., MERILH E.L., MERZOUGUI M., MESHKOV S., MESSENGER C., MESSICK C., METZDORFF R., MEYERS P.M., MEZZANI F., MIAO H., MICHEL C., MIDDLETON H., MIKHAILOV E.E., MILANO L., MILLER A.L., MILLER A., MILLER B.B., MILLER J., MILLHOUSE M., MINAZZOLI O., MINENKOV Y., MING J., MISHRA C., MITRA S., MITROFANOV V.P., MITSELMAKHER G., MITTLEMAN R., MOGGI A., MOHAN M., MOHAPATRA S.R.P., MONTANI M., MOORE B.C., MOORE C.J., MORARU D., MORENO G., MORRISS S.R., MOURS B., MOW-LOWRY C.M., MUELLER G., MUIR A.W., MUKHERJEE A., MUKHERJEE D., MUKHERJEE S., MUKUND N., MULLAVEY A., MUNCH J., MUNIZ E.A.M., MURRAY P.G., NAPIER K., NARDECCHIA I., NATICCHIONI L., NAYAK R.K., NELEMANS G., NELSON T.J.N., NERI M., NERY M., NEUNZERT A., NEWPORT J.M., NEWTON G., NG K.K.Y., NGUYEN T.T., NICHOLS D., NIELSEN A.B., NISSANKE S., NITZ A., NOACK A., NOCERA F., NOLTING D., NORMANDIN M.E.N., NUTTALL L.K., OBERLING J., OCHSNER E., OELKER E., OGIN G.H., OH J.J., OH S.H., OHME F., OLIVER M., OPPERMANN P., ORAM R.J., O'REILLY B., ORMISTON R., ORTEGA L.F., O'SHAUGHNESSY R., OTTAWAY D.J., OVERMIER H., OWEN B.J., PACE A.E., PAGE J., PAGE M.A., PAI A., PAI S.A., PALAMOS J.R., PALASHOV O., PALOMBA C., PAL-SINGH A., PAN H., PANG B., PANG P.T.H., PANKOW C., PANNARALE F., PANT B.C., PAOLETTI F., PAOLI A., PAPA M.A., PARIS H.R., PARKER W., PASCUCCI D., PASQUALETTI A., PASSAQUIETI R., PASSUELLO D., PATRICELLI B., PEARLSTONE B.L., PEDRAZA M., PEDURAND R., PEKOWSKY L., PELE A., PENN S., PEREZ C.J., PERRECA A., PERRI L.M., PFEIFFER H.P., PHELPS M., PICCINNI O.J., PICHOT M., PIERGIOVANNI F., PIERRO V., PILLANT G., PINARD L., PINTO I.M., PITKIN M., POGGIANI R., POPOLIZIO P., PORTER E.K., POST A., POWELL J., PRASAD J., PRATT J.W.W., PREDOI V., PRESTEGARD T., PRIJATELJ M., PRINCIPE M., PRIVITERA S., PRODI G.A., PROKHOROV L.G., PUNCKEN O., PUNTURO M., PUPPO P., PURRER M., QI H., QIN J., QIU S., QUETSCHKE V., QUINTERO E.A., QUITZOW-JAMES R., RAAB F.J., RABELING D.S., RADKINS H., RAFFAI P., RAJA S., RAJAN C., RAKHMANOV M., RAMIREZ K.E., RAPAGNANI P., RAYMOND V., RAZZANO M., READ J., REGIMBAU T., REI L., REID S., REITZE D.H., REW H., REYES S.D., RICCI F., RICKER P.M., RIEGER S., RILES K., RIZZO M., ROBERTSON N.A., ROBIE R., ROBINET F., ROCCHI A., ROLLAND L., ROLLINS J.G., ROMA V.J., ROMANO J.D., ROMANO R., ROMEL C.L., ROMIE J.H., ROSINSKA D., ROSS M.P., ROWAN S., RUDIGER A., RUGGI P., RYAN K., RYNGE M., SACHDEV S., SADECKI T., SADEGHIAN L., SAKELLARIADOU M., SALCONI L., SALEEM M., SALEMI F., SAMAJDAR A., SAMMUT L., SAMPSON L.M., SANCHEZ E.J., SANDBERG V., SANDEEN B., SANDERS J.R., SASSOLAS B., SATHYAPRAKASH B.S., SAULSON P.R., SAUTER O., SAVAGE R.L., SAWADSKY A., SCHALE P., SCHEUER J., SCHMIDT E., SCHMIDT J., SCHMIDT P., SCHNABEL R., SCHOFIELD R.M.S., SCHONBECK A., SCHREIBER E., SCHUETTE D., SCHULTE B.W., SCHUTZ B.F., SCHWALBE S.G., SCOTT J., SCOTT S.M., SEIDEL E., SELLERS D., SENGUPTA A.S., SENTENAC D., SEQUINO V., SERGEEV A., SHADDOCK D.A., SHAFFER T.J., SHAH A.A., SHAHRIAR M.S., SHAO L., SHAPIRO B., SHAWHAN P., SHEPERD A., SHOEMAKER D.H., SHOEMAKER D.M., SIELLEZ K., SIEMENS X., SIENIAWSKA M., SIGG D., SILVA A.D., SINGER A., SINGER L.P., SINGH A., SINGH R., SINGHAL A., SINTES A.M., SLAGMOLEN B.J.J., SMITH B., SMITH J.R., SMITH R.J.E., SON E.J., SONNENBERG J.A., SORAZU B., SORRENTINO F., SOURADEEP T., SPENCER A.P., SRIVASTAVA A.K., STALEY A., STEINKE M., STEINLECHNER J., STEINLECHNER S., STEINMEYER D., STEPHENS B.C., STEVENSON S.P., STONE R., STRAIN K.A., STRATTA G., STRIGIN S.E., STURANI R., STUVER A.L., SUMMERSCALES T.Z., SUN L., SUNIL S., SUTTON P.J., SWINKELS B.L., SZCZEPANCZYK M.J., TACCA M., TALUKDER D., TANNER D.B., TAPAI M., TARACCHINI A., TAYLOR J.A., TAYLOR R., THEEG T., THOMAS E.G., THOMAS M., THOMAS P., THORNE K.A., THORNE K.S., THRANE E., TIWARI S., TIWARI V., TOKMAKOV K.V., TOLAND K., TONELLI M., TORNASI Z., TORRIE C.I., TOYRA D., TRAVASSO F., TRAYLOR G., TRIFIRO D., TRINASTIC J., TRINGALI M.C., TROZZO L., TSANG K.W., TSE M., TSO R., TUYENBAYEV D., UENO K., UGOLINI D., UNNIKRISHNAN C.S., URBAN A.L., USMAN S.A., VAHI K., VAHLBRUCH H., VAJENTE G., VALDES G., VALLISNERI M., VAN BAKEL N., VAN BEUZEKOM M., VAN DEN BRAND J.F.J., VAN DEN BROECK C., VANDER-HYDE D.C., DER SCHAAF L., VAN HEIJNINGEN J.V., VAN VEGGEL A.A., VARDARO M., VARMA V., VASS S., VASUTH M., VECCHIO A., VEDOVATO G., VEITCH J., VEITCH P.J., VENKATESWARA K., VENUGOPALAN G., VERKINDT D., VETRANO F., VICERE A., VIETS A.D., VINCIGUERRA S., VINE D.J., VINET J., VITALE S., VO T., VOCCA H., VORVICK C., VOSS D.V., VOUSDEN W.D., VYATCHANIN S.P., WADE A.R., WADE L.E., WADE M., WALD R.M., WALET R., WALKER M., WALLACE L., WALSH S., WANG G., WANG H., WANG J.Z., WANG M., WANG Y., WARD R.L., WARNER J., WAS M., WATCHI J., WEAVER B., WEI L., WEINERT M., WEINSTEIN A.J., WEISS R., WEN L., WESSEL E.K., WESSELS P., WESTPHAL T., WETTE K., WHELAN J.T., WHITING B.F., WHITTLE C., WILLIAMS D., WILLIAMS R.D., WILLIAMSON A.R., WILLIS J.L., WILLKE B., WIMMER M.H., WINKLER W., WIPF C.C., WITTEL H., WOAN G., WOEHLER J., WOFFORD J., WONG K.W.K., WORDEN J., WRIGHT J.L., WU D.S., WU G., YAM W., YAMAMOTO H., YANCEY C.C., YAP M.J., YU H., YVERT M., ZADROZNY A., ZANOLIN M., ZELENOVA T., ZENDRI J., ZEVIN M., ZHANG L., ZHANG M., ZHANG T., ZHANG Y., ZHAO C., ZHOU M., ZHOU Z., ZHU X.J., ZIMMERMAN A., ZUCKER M.E., ZWEIZIG J.
	PhRvL, 118v, 1101 (2017)
	GW170104: observation of a 50-solar-mass binary black hole coalescence at redshift 0.2.
o	<GrW YYMMDD> (No. 170104).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GRZ88]
[GRZ88]	(Gonzalez-Riestra+Rego+Zamorano, 1988)
Write:	<<[GRZ88] Region A>>
N:	4
Object:	Region (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Calar Alto, INT observations. N=4 regions in Mrk 178: region A corresponds to the blue nucleus of Mrk 178. region B corresponds to the red fainter nucleus of Mrk 178. region C is a emission zone in the North. Region D is added in Fig.11 in 2003A&A...410..481N
in source:	Mrk 178
Ref:	=1988A&A...202...27G
by	GONZALEZ-RIESTRA R. , REGO M., ZAMORANO J.
	Astron. Astrophys., 202, 27-34 (1988)
	Star-forming knots in Mk 178.
o	Table 2, text: <[GRZ88] Region A> (Nos A-C).
Ref:	=2003A&A...410..481N
by	NOESKE K.G. , PAPADEROS P., CAIROS L.M., FRICKE K.J.
	Astron. Astrophys., 410, 481-509 (2003)
	New insights to the photometric structure of Blue Compact Dwarf galaxies from deep Near-Infrared studies. I. Observations, surface photometry and decomposition of surface brightness profiles.
o	Table 1 : Holmberg 263A = [H37] 263a. Fig.2: regions in Tol 3 = [SCK99] NGC 3125 A, B. Fig.8: regions 'MNN' = [ME99] Pox 4 NN. In reflist, Gonzalez-Riestra A&A.202 : the correct bibcode is 1988A&A.202.27G.
o	Fig.11: <[GRZ88] Region A> (Nos D) added. Figs 1, 5: <[NPC2003] UM 461 a> (Nos a-g). Fig.4: <[NPC2003] Haro 14 a> (Nos a-d). Fig.6: <[NPC2003] Hen 2-10 WW> (Nos E, W, NW). Fig.9: <[NPC2003] Tol 65 a> (Nos a-e). Fig.14: <[NPC2003] UM 448 a> (Nos a-c).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GS
GS	(GOODS South) (Not yet in Simbad)
*****	Avoid the usage of GS, prefer [LLH2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GS
GS	(Gal. Shell)
*****	Avoid the usage of GS, prefer [DGC92]
Details on Acronym: GS
GS	(Ginga Satellite)
*****	Avoid the usage of GS, prefer Ginga
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GS
GS	(Gaze+Shajn)
*****	Avoid the usage of GS, prefer [GS55]
Details on Acronym: GS
GS	(Gunn+Stryker)
*****	Avoid the usage of GS, prefer [GS83]
Origin	of the Acronym: L (1997MNRAS.289L..17J)
Details on Acronym: GS
GS	(Garnett+Shields)
*****	Avoid the usage of GS, prefer [GS87]
Origin	of the Acronym: L (1999ApJ...510..104B)
Details on Acronym: GS
GS	(Gal. Shell)
*****	Avoid the usage of GS, prefer GSH
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GS
GS	(Giant Shell)
*****	Avoid the usage of GS, prefer [KDS99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GS
GS	(Giant Shell)
*****	Avoid the usage of GS, prefer [MCW88]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GS
GS	(Gal. Shell)
*****	Avoid the usage of GS, prefer [W82]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GS2001]
[GS2001]	(Gibson+Stetson, 2001) (Not yet in Simbad)
Write:	<<[GS2001] CNN>>
N:	17
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
in source:	NGC 4527
Ref:	=2001ApJ...547L.103G
by	GIBSON B.K. , STETSON P.B.
	Astrophys. J., 547, 103-106 (2001)
	Supernova 1991T and the value of the Hubble constant.
o	Table 1:<[GS2001] CNN> (Nos C01-C16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GS2003]
[GS2003]	(Gil-Merino+Schindler, 2003)
Write:	<<[GS2003] JHHMMSS.s+DDMMSS.s>>
N:	1
Object:	AGN (SIMBAD class: AGN = Active Galaxy Nucleus)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of the galaxy cluster RBS 380: discovery of a bright AGN 'J030107.8-470624.0', probably the central cluster galaxy.
in source:	RBS 380
Ref:	=2003A&A...408...51G
by	GIL-MERINO R. , SCHINDLER S.
	Astron. Astrophys., 408, 51-56 (2003)
	Galaxy and hot gas distributions in the z=0.52 galaxy cluster RBS 380 from CHANDRA and NTT observations.
o	ClG 0050-24 is a misprint for ClG 0500-24.
o	Table 1: <[GS2003] JHHMMSS.s+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GS2005]
[GS2005]	(Gonzalez+Safi-Harb, 2005)
Write:	<<[GS2005] sNN>>
N:	18
Object:	* (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra CCD images of the field around the SNR 292.2-0.5. N=18 point sources are observed in the field.
Ref:	=2005ApJ...619..856G
by	GONZALEZ M. , SAFI-HARB S.
	Astrophys. J., 619, 856-862 (2005)
	Spatially resolved spectroscopy of the Chandra field containing the supernova remnant G292.2-0.5.
o	Table 2: <[GS2005] sNN> (Nos s1-s18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GS2007]
[GS2007]	(Gavazzi+Soucail, 2007)
Write:	<<[GS2007] Cl-NN>>
N:	14
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Weak lensing search of galaxy clusters in the 4 square degrees of the CFHT Legacy Survey Deep.
Ref:	=2007A&A...462..459G
by	GAVAZZI R. , SOUCAIL G.
	Astron. Astrophys., 462, 459-471 (2007)
	Weak lensing survey of galaxy clusters in the CFHTLS Deep.
o	Table 2: <[GS2007] Cl-NN> (Nos Cl-1 to Cl-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GS2008]
[GS2008]	(George+Stevens, 2008)= (GMRT)
Write:	<<[GS2008] JHHMMSS.s+DDMMSS>>
N:	113
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	GMRT 150MHz survey of a field centered on epsilon Eridani.
Ref:	=2008MNRAS.390..741G
by	GEORGE S.J. , STEVENS I.R.
	Mon. Not. R. Astron. Soc., 390, 741-751 (2008)
	A deep 150MHz Giant Metrewave Radio Telescope survey in Eridanus.
o	Table 1: <[GS2008] JHHMMSS.s+DDMMSS> N=113.
=E=	Catalogue in electronic form as J/MNRAS/390/741
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GS55]
[GS55]	(Gaze+Shajn, 1955)= (GS) = (HS)
Write:	<<[GS55] NNN>>
N:	286
Object:	Em. Nebula (SIMBAD class: ISM = Interstellar Medium Object)
Ref:	=1955IzKry..15...11G
by	GAZE V.F. , SHAJN G.A.
	Izv. Krym. Astrofiz. Obs., 15, 11-30 (1955)
	Catalogue of emission nebulae.
o	Table 1: <[GS55] NNN> (Nos 1-286)
Details on Acronym: [GS70]
[GS70]	(Goss+Shaver, 1970)
Write:	<<[GS70] LLL.l+B.b>> <<[GS70] LLL.l+BB.b>>
N:	206
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Observations at 5000MHz of N=206 galactic radio-sources. See also paper II: [SG70].
Ref:	=1970AuJPA..14....1G
by	GOOS W.H. , SHAVER P.A.
	Australian J. Phys. Astrophys. Suppl., 14, 1-75 (1970)
	Galactic radio sources : 5000 MHz observations, 408 MHz observations, spectra, physical characteres.
o	Table 1: <[GS70] LLL.l+B.b>, <[GS70] LLL.l+BB.b>, N=206.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GS80]
[GS80]	(Gopal-Krishna+Sramek, 1980)
Write:	<<[GS80] PHL 938 source N>> <<[GS80] PHL 5200 A>>
N:	3+3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=3 radio-sources in the field of PHL 938. N=3, a triple radio-source, surrounding PHL 5200.
Ref:	=1980A&A....90L...1G
by	GOPAL-KRISHNA , SRAMEK R.A.
	Astron. Astrophys., 90, 1-3 (1980)
	VLA observations of the absorption-line quasars PHL 938 and PHL 5200.
o	Elliptical galaxy in the field of PHL 938 = [WBP78] Object 1.
o	Text: <[GS80] PHL 938 source N> (Nos 1-3). Fig.1: <[GS80] PHL 5200 A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GS83]
[GS83]	(Gunn+Stryker, 1983)= (BPGS) = (GS)
Write:	<<[GS83] NNN>>
N:	175
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Spectrophotometric catalogue of 175 stars covering a complete range of spectral types and luminosity classes. The Bruzual-Persson-Gunn-Stryker (BPGS) Spectral Atlas, is an extension of the Gunn & Stryker (1983) optical atlas ranging from the UV to the near-IR.
Ref:	=1983ApJS...52..121G
by	GUNN J.E. , STRYKER L.L.
	Astrophys. J., Suppl. Ser., 52, 121-153 (1983)
	Stellar spectrophotometric Atlas, 3130 <λ <10800 A.
o	Table 1: <[GS83] NNN> (Nos 1-175)
=E=	Catalogue in electronic form as III/88
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GS84]
[GS84]	(Gopal-Krishna+Saripalli, 1984)
Write:	<<[GS84] Aw>>
N:	4+4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Fig.1: Radio peaks in Cen A, northern peaks with a format 'An', and their southern counterparts format 'As'.
in source:	Cen A = NGC 5128
Ref:	=1984A&A...141...61G
by	GOPAL-KRISHNA , SARIPALLI L.
	Astron. Astrophys., 141, 61-66 (1984)
	Possible relationship between the radio and optical structures associated with the active galaxy Centaurus A.
o	Fig.2: Object G = BGLO Cen A Knot G.
o	Fig.1: <[GS84] Aw> (Nos An to Dn, As to Ds).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GS87]
[GS87]	(Garnett+Shields, 1987)= (GS) = ([LL87])
Write:	<<[GS87] NN>>
N:	13 among 17
Object:	HII (SIMBAD class: HIIReg = HII Region)
in source:	M 81 = NGC 3031
Ref:	=1987ApJ...317...82G
by	GARNETT D.R. , SHIELDS G.A.
	Astrophys. J., 317, 82-101 (1987)
	The composition gradient across M 81.
o	Munch = [M59b] in SIMBAD. Numbering 'NN' is from a survey of Leisawitz+Levreault, 1987, not published
o	Tables 1, 2: <[GS87] NN> N=13 among (Nos 1-17).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GS98]
[GS98]	(Germany+Sabine, 1998)
Write:	<<[GS98] JHHMMSS.ss+DDMMSS.s>>
N:	1+1
Object:	G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=1 Host galaxy of SN 1998EZ: J035732.88-271217.6 N=1 nearby star in the field: J035730.25-271116.1
Ref:	=1998IAUC.7070Q...1G
by	GERMANY L. , SABINE S.
	IAU Circ., 7070, 1-None (1998)
	Supernova 1998ez in anonymous galaxy.
o	<[GS98] J035732.88-271217.6>, <[GS98] J035730.25-271116.1>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GSA
GSA	(G, South, field A)
Write:	<<GSA NNNA>>
N:	140
Object:	G (SIMBAD class: Galaxy)
Note:	Anglo Australian Redshift Survey (AARS). See also GNA, GNB, GSAN, GSD, GSF
Ref:	=1986MNRAS.221..233P
by	PETERSON B.A. , ELLIS R.S., EFSTATHIOU G., SHANKS T., BEAN A.J., FONG R., ZEN-LONG Z.
	Mon. Not. R. Astron. Soc., 221, 233-255 (1986)
	A complete galaxy redshift sample - III. Methods and catalogue.
o	Table 3: <GSA NNNA> N=140 among (Nos 1-137), <GSAN N> (Nos 1-5), <GSD NNN> N=128 among (Nos 1-179), <GSF NNN> N=78 among (Nos 1-100), <GNA NN> N=80 among (Nos 1-81), <GNB NN> N=94 among (Nos 1-95)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GSA2000]
[GSA2000]	(Geller+Sault+Antonucci+, 2000) (Not yet in Simbad)
Write:	<<[GSA2000] a>>
N:	5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	N=5 brightest sources in the field of QSO 1935-692. Finding chart in Fig.2.
Ref:	=2000ApJ...539...73G
by	GELLER R.M. , SAULT R.J., ANTONUCCI R., KILLEEN N.E.B., EKERS R., DESAI K., WHYSONG D.
	Astrophys. J., 539, 73-88 (2000)
	Cosmological halos: a search for the ionized intergalactic medium.
o	Table 2: <[GSA2000] a> (Nos a-e).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSA2019]
[GSA2019]	(Gburek+Siana+Alavi+, 2019)
Write:	<<[GSA2019] A1689-217>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck I MOSFIRE and LRIS observations of N=1 star-forming dwarf galaxy, lensed by the galaxy cluster ACO 1689.
in source:	ACO 1689
Ref:	=2019ApJ...887..168G
by	GBUREK T. , SIANA B., ALAVI A., EMAMI N., RICHARD J., FREEMAN W.R., STARK D.P., SNAPP-KOLAS C., LUCERO B.
	Astrophys. J., 887, 168-168 (2019)
	The detection of [O III] λ4363 in a lensed, Dwarf galaxy at z = 2.59: testing metallicity indicators and scaling relations at high redshift and Low mass.
o	Fig. 1, Tables 1-2: <[GSA2019] A1689-217> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GSAN
GSAN	(G, South, field AN)
Write:	<<GSAN N>>
N:	5
Object:	G (SIMBAD class: Galaxy)
Note:	Anglo Australian Redshift Survey (AARS). See also GNA, GNB, GSA, GSD, GSF
Ref:	=1986MNRAS.221..233P
by	PETERSON B.A. , ELLIS R.S., EFSTATHIOU G., SHANKS T., BEAN A.J., FONG R., ZEN-LONG Z.
	Mon. Not. R. Astron. Soc., 221, 233-255 (1986)
	A complete galaxy redshift sample - III. Methods and catalogue.
o	Table 3: <GSA NNNA> N=140 among (Nos 1-137), <GSAN N> (Nos 1-5), <GSD NNN> N=128 among (Nos 1-179), <GSF NNN> N=78 among (Nos 1-100), <GNA NN> N=80 among (Nos 1-81), <GNB NN> N=94 among (Nos 1-95)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GSB2003]
[GSB2003]	(Goudfrooij+Strader+Brenneman+, 2003)= ([GSB2003a])
Write:	<<[GSB2003] 3628-NN>> <<[GSB2003] 4013-NN>> <<[GSB2003] 4517-NN>> <<[GSB2003] 5176-NN>> <<[GSB2003] 7814-NN>>
N:	50+50+50+50+17
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	HST WFPC2 observations: phtometry and astrometry of the 50 brightest globular cluster candidates in 5 galaxies. (In NGC 7814, only 17 GCl).
in source:	NGC 3628
in source:	NGC 4013
in source:	NGC 4517
in source:	IC 5176
in source:	NGC 7814
Ref:	=2003MNRAS.343..665G
by	GOUDFROOIJ P. , STRADER J., BRENNEMAN L., KISSLER-PATIG M., MINNITI D., HUIZINGA J.E.
	Mon. Not. R. Astron. Soc., 343, 665-678 (2003)
	Hubble Space Telescope observations of globular cluster systems along the Hubble sequence of spiral galaxies.
o	Table B1: <[GSB2003] 3628-NN> (Nos 1-50). Table B2: <[GSB2003] 4013-NN> (Nos 1-50). Table B3: <[GSB2003] 4517-NN> (Nos 1-50). Table B4: <[GSB2003] 5176-NN> (Nos 1-50). Table B5: <[GSB2003] 7814-NN> (Nos 1-17).
=E=	Catalogue in electronic form as J/MNRAS/343/665
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSB2003a]
[GSB2003a]	(Goudfrooij+Strader+Brenneman+, 2003) (Not yet in Simbad)
*****	Avoid the usage of [GSB2003a], prefer [GSB2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSB2003b]
[GSB2003b]	(Gliozzi+Sambruna+Brandt, 2003)
Write:	<<[GSB2003b] A>>
N:	5
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-S images of NGC 4261: N=5 off-nuclear X-ray point-like sources.
in source:	NGC 4261
Ref:	=2003A&A...408..949G
by	GLIOZZI M. , SAMBRUNA R.M., BRANDT W.N.
	Astron. Astrophys., 408, 949-959 (2003)
	On the origin of the X-rays and the nature of accretion in NGC 4261.
o	Table 4: <[GSB2003b] A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSB2009]
[GSB2009]	(Guzzo+Schuecker+Boehringer+, 2009)
Write:	<<[GSB2009] JHHMMSS.ss+DDMMSS.s>>
N:	1267
Object:	Unknown (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Spectroscopic observations (with ESO 1.5m, 2m and 3.6m telescopes) of clusters from the ROSAT-ESO Flux-Limited X-ray (REFLEX) catalog of galaxy clusters.
Ref:	=2009A&A...499..357G
by	GUZZO L. , SCHUECKER P., BOEHRINGER H., COLLINS C.A., ORTIZ-GIL A., DE GRANDI S., EDGE A.C., NEUMANN D.M., SCHINDLER S., ALTUCCI C., SHAVER P.A.
	Astron. Astrophys., 499, 357-369 (2009)
	The REFLEX galaxy cluster survey. VIII. Spectroscopic observations and optical atlas.
o	Table 2: <[GSB2009] JHHMMSS.ss+DDMMSS.s> N=1267.
=E=	Catalogue in electronic form as J/A+A/499/357
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSB2010]
[GSB2010]	(Gupta+Srianand+Bowen+, 2010)
Write:	<<[GSB2010] G1>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Galaxy near QSO-galaxy pair. Use of SDSS DR5 data.
Ref:	=2010MNRAS.408..849G
by	GUPTA N. , SRIANAND R., BOWEN D.V., YORK D.G., WADADEKAR Y.
	Mon. Not. R. Astron. Soc., 408, 849-864 (2010)
	GMRT mini-survey to search for 21-cm absorption in quasar-galaxy pairs at z ~ 0.1.
o	Fig. 7 and text: <[GSB2010] G1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSB2014]
[GSB2014]	(Gruen+Seitz+Brimioulle+, 2014) (Not yet in Simbad)
Write:	<<[GSB2014] SPT-CL JHHMM+DDMM A>> <<[GSB2014] PLCKESZ GLLL.l+BB.b A>> <<[GSB2014] MACS J0416.1-2403 A>> <<[GSB2014] PSZ1 GLLL.ll+BB.bb A>>
N:	14+6+3+9
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	N=32 secondary clusters and groups in the fields of ten clusters of galaxies selected for the Sunyaev-Zel'dovich (SZ) effect.
Ref:	=2014MNRAS.442.1507G
by	GRUEN D. , SEITZ S., BRIMIOULLE F., KOSYRA R., KOPPENHOEFER J., LEE C.-H., BENDER R., RIFFESER A., EICHNER T., WEIDINGER T., BIERSCHENK M.
	Mon. Not. R. Astron. Soc., 442, 1507-1544 (2014)
	Weak lensing analysis of SZ-selected clusters of galaxies from the SPT and Planck surveys.
o	Table A1: <[GSB2014] SPT-CL JHHMM+DDMM A> N=14, <[GSB2014] PLCKESZ GLLL.l+BB.b A> N=6, <[GSB2014] MACS J0416.1-2403 A> N=3, <[GSB2014] PSZ1 GLLL.ll+BB.bb A> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSB2021]
[GSB2021]	(Gudin+Shank+Beers+, 2021) (Not yet in Simbad)
Write:	<<[GSB2021] CDTG-NN>>
N:	30
Object:	Stellar Group (SIMBAD class: Cluster* = Cluster of Stars)
Note:	N=30 chemodynamically tagged groups (CDTGs) of metal-poor stars in the halo and disk systems of the Milky Way.
Ref:	=2021ApJ...908...79G
by	GUDIN D. , SHANK D., BEERS T.C., YUAN Z., LIMBERG G., ROEDERER I.U., PLACCO V., HOLMBECK E.M., DIETZ S., RASMUSSEN K.C., HANSEN T.T., SAKARI C.M., EZZEDDINE R., FREBEL A.
	Astrophys. J., 908, 79-79 (2021)
	The r-process Alliance: chemodynamically tagged groups of halo r-process-enhanced stars reveal a shared chemical-evolution history.
o	Tables 5-6: <[GSB2021] CDTG-NN> (Nos 1-30).
o	Substructures from table 8 and CDTGs groups from table 6 are not in SIMBAD.
=E=	Catalogue in electronic form as <J/ApJ/908/79/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GSC
GSC	(Gas-Star Complex)
*****	Avoid the usage of GSC, prefer [DS95]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GSC
GSC	(Guide Star Catalog)= (HSTGC)
Write:	<<GSC FFFFF-NNNNN>>
N:	about 25000000
Object:	* (SIMBAD class: Star)
Note:	The Guide Star Catalog (GSC) has been constructed to support the operational requirement of the Hubble Space Telescope for off-axis stars. It contains approximately 1.9x10(7) stars and other objects in the sixth to fifteenth magnitude range. In the format 'FFFFF' stands for an internal region number. Format FFFFF0NNNNN is also often found in the literature.
Ref:	=1990AJ.....99.2019L
by	LASKER B.M. , STURCH C.R., McLEAN B.J., RUSSELL J.L., JENKNER H., SHARA M.M.
	Astron. J., 99, 2019-2058 (1990)
	The Guide Star Catalog. I. Astronomical foundations and image processing.
o	Description of the GSC catalogue, no object in the reference.
o	<GSC FFFFF-NNNNN>
Ref:	=1990AJ.....99.2059R
by	RUSSELL J.L. , LASKER B.M., McLEAN B.J., STURCH C.R., JENKNER H.
	Astron. J., 99, 2059-2081 (1990)
	The Guide Star Catalog. II. Photometric and astrometric models and solutions.
o	Description of the GSC catalogue, no object in the reference.
o	<GSC FFFFF-NNNNN>
Ref:	=1990AJ.....99.2082J
by	JENKNER H. , LASKER B.M., STURCH C.R., McLEAN B.J., SHARA M.M., RUSSELL J.L.
	Astron. J., 99, 2082-2154 (1990)
	The Guide Star Catalog. III. Production, database organisation, and population statistics.
o	Description of the GSC catalogue, no object in the reference.
o	<GSC FFFFF-NNNNN>
Ref:	=1990GSC1..C......0L
by	LASKER B.M. , et al.
	The HST Guide Star Catalog Version 1.1, 0-None (1990)
	An all-sky astrometric and photometric catalogue to support the operation of the Hubble Space Telescope.
o	<GSC FFFFF-NNNNN>
Ref:	=2001AJ....121.1752M
by	MORRISON J.E. , ROESER S., McLEAN B., BUCCIARELLI B., LASKER B.
	Astron. J., 121, 1752-1763 (2001)
	The Guide Star Catalog, version 1.2: an astrometric recalibration and other refinements.
o	<GSC FFFFF-NNNNN>
=E=	Catalogue in electronic form as I/220
=E=	Catalogue in electronic form as I/254
=E=	Catalogue in electronic form as I/255
Origin	of the Acronym: L = Found in the literature
Details on Acronym: GSC2.2
GSC2.2	(Guide Star Catalog, version 2.2)
Write:	<<GSC2 WNNNNNNNNNNNNN>>
N:	455851237
Object:	* (SIMBAD class: Star)
Note:	The GSC2.2 is a preliminary version of GSC II generated to support telescope operations at the GEMINI and VLT telescopes.
Ref:	=2001yCat.1271....0S
by	SPACE TELESCOPE SCIENCE INSTITUTE , (The Osservatorio Astronomico di Torino)
	CDS/ADC Collection of Electronic Catalogues, -1-None (2001)
	The Guide Star Catalog, Version 2.2 (GSC2.2).
o	<GSC2.2 WNNNNNNNNNNNNN> N=455851237.
=E=	Catalogue in electronic form as I/271
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GSC2.3
GSC2.3	(Guide Star Catalog, version 2.3)
Write:	<<GSC2.3 {N\|S}{A..Z\|0..9}{A..Z\|0..9}{A..Z\|0..9}{A..Z\|0..9}NNNNNN>>
Object:	* (SIMBAD class: Star)
Note:	GSC II all-sky catalog. The GSC2.3 identification differs from GSC2.2 preliminary version: 10 characters, the first four representing the level-6 HTM (Hierarchical Triangular Mesh) coded in base 36 (0..9 and A..Z), and the last 6 represent a zero-filled sequence number assigned to each source upon initial detection.
Auth.:	Space Telescope Science Institute+
=E=	Catalogue in electronic form as I/305
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GSC2007]
[GSC2007]	(Geach+Smail+Chapman+, 2007)= (LAB)
Write:	<<[GSC2007] LAB NNa>>
N:	5+3+2
Object:	(Mid IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Spitzer Space Telescope IRAC and MIPS images and HST observations of the 2 Lyman-alpha emitting blobs or nebulae [TSK2001] LAB 1 and 2.
in source:	[TSK2001] LAB 1 = [MYH2004] LAB 1
in source:	[TSK2001] LAB 2 = [MYH2004] LAB 2
in source:	[MYH2004] LAB 18
Ref:	=2007ApJ...655L...9G
by	GEACH J.E. , SMAIL I., CHAPMAN S.C., ALEXANDER D.M., BLAIN A.W., STOTT J.P., IVISON R.J.
	Astrophys. J., 655L, 9-12 (2007)
	Spitzer identifications and classifications of submillimeter galaxies in giant, high-redshift, Lyα-Emission-Line nebulae.
o	Fig.1, Table 1: <[GSC2007] LAB 1a> (Nos 1a-1e), <[GSC2007] LAB 2a> (Nos 2a-2c).
Ref:	=2009ApJ...692.1561W
by	WEBB T.M.A. , YAMADA T., HUANG J.-S., ASHBY M.L.N., MATSUDA Y., EGAMI E., GONZALEZ M., HAYASHINO T.
	Astrophys. J., 692, 1561-1570 (2009)
	Spitzer observations of extended Lyman-α clouds in the SSA22 field.
o	Table 1: <[GSC2007] LAB NNa> (Nos 18a, 18b) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSC2021]
[GSC2021]	(Graham+Soria+Ciambur+, 2021)
Write:	<<[GSC2021] Nikhuli>> <<[GSC2021] NGC 4424 X-3>>
N:	1+1
Object:	Cluster of * + (X) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=1 infalling star cluster and N=1 X-ray source near the center of NGC 4424. Use of HST and Chandra archival data, and of data from the Next Generation Virgo Cluster Survey.
in source:	NGC 4424
Ref:	=2021ApJ...923..146G
by	GRAHAM A.W. , SORIA R., CIAMBUR B.C., DAVIS B.L., SWARTZ D.A.
	Astrophys. J., 923, 146-146 (2021)
	Potential black hole seeding of the spiral galaxy NGC 4424 via an infalling star cluster.
o	<[GSC2021] Nikhuli> N=1. Fig. 3: <[GSC2021] NGC 4424 X-3> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GSC2U
GSC2U	(Guide Star Catalogue, Version 2, Unregistered)
Write:	<<GSC2U JHHMMSS.s+DDMMSS>>
N:	41
Object:	WD* (SIMBAD class: WhiteDwarf = White Dwarf)
Note:	GSC-II white Dwarf survey.
Ref:	=2006A&A...448..579C
by	CAROLLO D. , BUCCIARELLI B., HODGKIN S.T., LATTANZI M.G., McLEAN B., MORBIDELLI R., SMART R.L., SPAGNA A., TERRANEGRA L.
	Astron. Astrophys., 448, 579-588 (2006)
	The GSC-II-based survey of ancient cool white dwarfs. I. The sample of spectroscopically confirmed white dwarfs.
o	GSC2U J133360.0+001654 is GSC2U J133400.0+001654 in Simbad. Paragraph 4 . SP stars not identified.
o	Table 2: <GSC2U JHHMMSS.s+DDMMSS> N=41.
=E=	Catalogue in electronic form as J/A+A/448/579
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GSD
GSD	(G, South, field D)
Write:	<<GSD NNN>>
N:	128
Object:	G (SIMBAD class: Galaxy)
Note:	Anglo Australian Redshift Survey (AARS). See also GNA, GNB, GSA, GSAN, GSF
Ref:	=1986MNRAS.221..233P
by	PETERSON B.A. , ELLIS R.S., EFSTATHIOU G., SHANKS T., BEAN A.J., FONG R., ZEN-LONG Z.
	Mon. Not. R. Astron. Soc., 221, 233-255 (1986)
	A complete galaxy redshift sample - III. Methods and catalogue.
o	Table 3: <GSA NNNA> N=140 among (Nos 1-137), <GSAN N> (Nos 1-5), <GSD NNN> N=128 among (Nos 1-179), <GSF NNN> N=78 among (Nos 1-100), <GNA NN> N=80 among (Nos 1-81), <GNB NN> N=94 among (Nos 1-95)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GSD2012]
[GSD2012]	(Gouliermis+Schmeja+Dolphin+, 2012)
Write:	<<[GSD2012] NN>>
N:	14
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	N=14 sub-clusters in the region NGC 602 and LHA 115-N90. Use of HST ACS archival data.
Ref:	=2012ApJ...748...64G
by	GOULIERMIS D.A. , SCHMEJA S., DOLPHIN A.E., GENNARO M., TOGNELLI E., PRADA MORONI P.G.
	Astrophys. J., 748, 64 (2012)
	The clustered nature of star formation. Pre-main-sequence clusters in the star-forming region NGC 602/N90 in the Small Magellanic Cloud.
o	Fig. 6, Table 1: <[GSD2012] NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSD2013]
[GSD2013]	(Gusev+Sakhibov+Dodonov, 2013)= ([GSD2013a])
Write:	<<[GSD2013] NN>>
N:	39
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	SAO 6m BTA telescope SCORPIO observations of N=39 HII regions in the spiral galaxy NGC 6946.
in source:	NGC 6946
Ref:	=2013AstBu..68...40G
by	GUSEV A.S. , SAKHIBOV F.H., DODONOV S.N.
	AstBu, 68, 40 (2013)
	Spectroscopy of H II regions in the late-type spiral galaxy NGC 6946.
o	Fig. 2, Table 3: <[GSD2013] NN> (Nos 1-39).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSD2013a]
[GSD2013a]	(Gusev+Sakhibov+Dodonov, 2013)
*****	Avoid the usage of [GSD2013a], prefer [GSD2013]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSD2013b]
[GSD2013b]	(Gobat+Strazzullo+Daddi+, 2013)
Write:	<<[GSD2013b] NNNNN>> <<[GSD2013b] NNNN.N>>
N:	27
Object:	G (SIMBAD class: Galaxy)
Note:	HST WFC3 slitless spectroscopic observations of N=27 galaxies of the distant cluster Cl J1449+0856.
in source:	ClG J1449+0856
Ref:	=2013ApJ...776....9G
by	GOBAT R. , STRAZZULLO V., DADDI E., ONODERA M., CAROLLO M., RENZINI A., FINOGUENOV A., CIMATTI A., SCARLATA C., ARIMOTO N.
	Astrophys. J., 776, 9 (2013)
	WFC3 GRISM confirmation of the distant cluster Cl J1449+0856 at $ < z$ > = 2.00: quiescent and star-forming galaxy populations.
o	Table 2: <[GSD2013b] NNNNN> N=25 among (Nos 41-22111), Table 2: <[GSD2013b] NNNN.N> N=2 (Nos 141.2, 1411.3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSD97]
[GSD97]	(Gao+Solomon+Downes+, 1997) (Not yet in Simbad)
Write:	<<[GSD97] NN>>
N:	13
Object:	CO source (SIMBAD class: Cloud)
Note:	N=13 CO sources in NGC 1144. See also [ACG2003].
in source:	NGC 1144
Ref:	=2003ApJ...586..939C
by	CHANDAR R. , LEITHERER C., TREMONTI C., CALZETTI D.
	Astrophys. J., 586, 939-958 (2003)
	The stellar content of Henize 2-10 from Space Telescope Imaging Spectrograph ultraviolet spectroscopy.
o	Table 1: <[CLT2003] Cluster N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSE2009]
[GSE2009]	(Gliozzi+Satyapal+Eracleous+, 2009)
Write:	<<[GSE2009] AN>>
N:	3+2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS and VLA observations of NGC 3621. Use of Spitzer IRAC data.
in source:	NGC 3621
Ref:	=2009ApJ...700.1759G
by	GLIOZZI M. , SATYAPAL S., ERACLEOUS M., TITARCHUK L., CHEUNG C.C.
	Astrophys. J., 700, 1759-1767 (2009)
	A Chandra view of NGC 3621: a bulgeless galaxy hosting an AGN in its early phase?
o	Fig. 2: <[GSE2009] A> (Nos A-C). Fig. 7: <[GSE2009] AN> (Nos C1-C2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GSF
GSF	(G, South, field F)
Write:	<<GSF NNN>>
N:	78
Object:	G (SIMBAD class: Galaxy)
Note:	Anglo Australian Redshift Survey (AARS). See also GNA, GNB, GSA, GSAN, GSD
Ref:	=1986MNRAS.221..233P
by	PETERSON B.A. , ELLIS R.S., EFSTATHIOU G., SHANKS T., BEAN A.J., FONG R., ZEN-LONG Z.
	Mon. Not. R. Astron. Soc., 221, 233-255 (1986)
	A complete galaxy redshift sample - III. Methods and catalogue.
o	Table 3: <GSA NNNA> N=140 among (Nos 1-137), <GSAN N> (Nos 1-5), <GSD NNN> N=128 among (Nos 1-179), <GSF NNN> N=78 among (Nos 1-100), <GNA NN> N=80 among (Nos 1-81), <GNB NN> N=94 among (Nos 1-95)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GSF2000]
[GSF2000]	(Gibson+Stetson+Freedman+, 2000)
Write:	<<[GSF2000] NGC NNNN CNN>> <<[GSF2000] NGC NNNNA CNN>> <<[GSF2000] IC NNNN CNN>>
N:	17+39+36+11+7+28+94
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Note:	HST observations. Search for cepheids in 7 galaxies. See also: [FHM94], [HST94], [KIF96], [FFH96], [SHM96], [GPF97], [RMM97], [FBK98], [HHH98], [PSF98], [TFS98], [GHS99], [KIS99], [SHF99], [GFF99], [MHS99], [PBK99], [SFK99], [MHS2000]
in source:	NGC 4639
in source:	NGC 4536
in source:	NGC 3627
in source:	NGC 3368
in source:	NGC 5253
in source:	IC 4182
in source:	NGC 4496A
Ref:	=2000ApJ...529..723G
by	GIBSON B.K. , STETSON P.B., FREEDMAN W.L., MOULD J.R., KENNICUTT R.C.Jr, HUCHRA J.P., SAKAI S., GRAHAM J.A., FASSETT C.I., KELSON D.D., FERRARESE L., HUGHES S.M.G., ILLINGWORTH G.D., MACRI L.M., MADORE B.F., SEBO K.M., SILBERMANN N.A.
	Astrophys. J., 529, 723-744 (2000)
	The Hubble space telescope key project on the extragalactic distance scale. XXV. A recalibration of cepheid distances to type Ia supernovae and the value of the Hubble constant.
o	Table A1: <[GSF2000] NGC 4639 CNN> (Nos C1-C17). Table A2: <[GSF2000] NGC 4536 CNN> (Nos C1-C39). Table A3: <[GSF2000] NGC 3627 CNN> (Nos C1-C36). Table A4: <[GSF2000] NGC 3368 CNN> (Nos C1-C11). Table A5: <[GSF2000] NGC 5253 CN> (Nos C1-C7). Table A6: <[GSF2000] IC 4182 CNN> (Nos C1-C28). Table A7: <[GSF2000] NGC 4496A CNN> (Nos C1-C94).
=E=	Catalogue in electronic form as J/ApJ/529/723
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSF2004]
[GSF2004]	(Gillmon+Sanders+Fabian, 2004)
Write:	<<[GSF2004] JHHMMSS.ss+DDMMSS.s>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observation of NGC 1275. N=2 point sources are detected.
Ref:	=2004MNRAS.348..159G
by	GILLMON K. , SANDERS J.S., FABIAN A.C.
	Mon. Not. R. Astron. Soc., 348, 159-164 (2004)
	An X-ray absorption analysis of the high-velocity system in NGC 1275.
o	Text: <[GSF2004] JHHMMSS.ss+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSF2010]
[GSF2010]	(Giodini+Smolcic+Finoguenov+, 2010)
Write:	<<[GSF2010] NNNa>>
N:	16+7+15+11
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	Observations of galaxy groups from the GEEC (Group Environment Evolution Collaboration) spectroscopic survey. More information available at http://quixote.uwaterloo.ca/~mbalogh/research/GEEC/
Ref:	=2010ApJ...714..218G
by	GIODINI S. , SMOLCIC V., FINOGUENOV A., BOEHRINGER H., BIRZAN L., ZAMORANI G., OKLOPCIC A., PIERINI D., PRATT G.W., SCHINNERER E., MASSEY R., KOEKEMOER A.M., SALVATO M., SANDERS D.B., KARTALTEPE J.S., THOMPSON D.
	Astrophys. J., 714, 218-228 (2010)
	Radio galaxy feedback in x-ray-selected groups from COSMOS: the effect on the intracluster medium.
o	Table 1: <[GSF2010] NNN> N=16 among (Nos 6-311).
Ref:	=2011MNRAS.412.2303B
by	BALOGH M.L. , McGEE S.L., WILMAN D.J., FINOGUENOV A., PARKER L.C., CONNELLY J.L., MULCHAEY J.S., BOWER R.G., TANAKA M., GIODINI S.
	Mon. Not. R. Astron. Soc., 412, 2303-2317 (2011)
	Direct observational evidence for a large transient galaxy population in groups at 0.85 < z < 1.
o	Table 1: <[GSF2010] NNNa> N=7 among (Nos 40-213a).
Ref:	=2012MNRAS.421.3594H
by	HOU A. , PARKER L.C., WILMAN D.J., McGEE S.L., HARRIS W.E., CONNELLY J.L., BALOGH M.L., MULCHAEY J.S., BOWER R.G.
	Mon. Not. R. Astron. Soc., 421, 3594-3611 (2012)
	Substructure in the most massive GEEC groups: field-like populations in dynamically active groups.
o	Tables 2-3:<[GSF2010] NNNa> N=4+11 among (Nos 4-362).
Ref:	=2013MNRAS.431.1090M
by	MOK A. , BALOGH M.L., McGEE S.L., WILMAN D.J., FINOGUENOV A., TANAKA M., GIODINI S., BOWER R.G., CONNELLY J.L., HOU A., MULCHAEY J.S., PARKER L.C.
	Mon. Not. R. Astron. Soc., 431, 1090-1106 (2013)
	Efficient satellite quenching at z ~ 1 from the GEEC2 spectroscopic survey of galaxy groups.
o	Table 1: <[GSF2010] NNNa> N=11 among (Nos 40-213a).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSF2018]
[GSF2018]	(Gonzalez+Smith Castelli+Faifer+, 2018)
Write:	<<[GSF2018] PEG JHHMMSS+DDMMSS.s>>
N:	8
Object:	LSB (SIMBAD class: LowSurfBrghtG = Low Surface Brightness Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Gemini North GMOS photometric observations of N=8 low-surface-brightness (LSB) galaxies in the central region of Pegasus I.
in source:	NAME Peg I
Ref:	=2018A&A...620A.166G
by	GONZALEZ N.M. , SMITH CASTELLI A.V., FAIFER F.R., ESCUDERO C.G., CELLONE S.A.
	Astron. Astrophys., 620A, 166-166 (2018)
	Stellar systems in the direction of Pegasus I. I. Low surface brightness galaxies.
o	Tables 3-4: <[GSF2018] PEG JHHMMSS+DDMMSS.s> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSF98]
[GSF98]	(Gaensler+Stappers+Frail+, 1998)= (ATCA) = (PWN)
Write:	<<[GSF98] PWN BHHMM+DD>> <<[GSF98] ATCA JHHMMSS+DDMMSS>>
N:	2
Object:	Nebula (SIMBAD class: ISM = Interstellar Medium Object)
Stat:	is completely incorporated in Simbad
Note:	ATCA observations of the old pulsar PSR 0906-49: N=1 source, coincident with the PSR, interpreted as the Pulsar Wind Nebula, format 'PWN B0906-49'. and N=1 unrelated source, format 'ATCA J090850-491301'
Ref:	=1998ApJ...499L..69G
by	GAENSLER B.M. , STAPPERS B.W., FRAIL D.A., JOHNSTON S.
	Astrophys. J., 499, 69-74 (1998)
	An unusual pulsar wind nebula associated with PSR B0906-49.
o	Table 2: <[GSF98] PWN B0906-49> N=1, <[GSF98] ATCA J090850-491301> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GSG
GSG	(G, South, field G)
Write:	<<GSG NNN>>
N:	159
Object:	G (SIMBAD class: Galaxy)
Ref:	=1989MNRAS.236..207M
by	METCALFE N. , FONG R., SHANKS T., KILKENNY D.
	Mon. Not. R. Astron. Soc., 236, 207-234 (1989)
	An extended galaxy redshift survey - I. The catalogue.
o	<GNH NNN> (Nos 1-106), <GNX NNN> (Nos 1-113), <GNY NN> (Nos 1-91), <GNZ NNN> (Nos 1-130), <GSG NNN> (Nos 1-159), <GSI NNN> (Nos 1-136), <GSM NNN> (Nos 1-130), <GSN NNN> (Nos 1-195), <GSP NN> (Nos 1-74)
=E=	Catalogue in electronic form as J/MNRAS/236/207
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GSG2007]
[GSG2007]	(Goudfrooij+Schweizer+Gilmore+, 2007)
Write:	<<[GSG2007] GNN>>
N:	50
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations of NGC 3610 to search for globular clusters.
in source:	NGC 3610
Ref:	=2007AJ....133.2737G
by	GOUDFROOIJ P. , SCHWEIZER F., GILMORE D., WHITMORE B.C.
	Astron. J., 133, 2737-2751 (2007)
	Dynamical evolution of globular cluster systems formed in galaxy mergers: deep Hubble Space Telescope advanced camera for surveys imaging of old and intermediate-age globular clusters in NGC 3610.
o	Table 1: <[GSG2007] GNN> (Nos G1-G50).
=E=	Catalogue in electronic form as J/AJ/133/2737
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSG2009]
[GSG2009]	(Ghosh+Saripalli+Poshak+, 2009)
Write:	<<[GSG2009] NN>>
N:	49
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS and XMM-Newton observations of the interacting pair of galaxies NGC 5774/5775.
in source:	NGC 5774
in source:	NGC 5775
Ref:	=2009AJ....137.3263G
by	GHOSH K.K. , SARIPALLI L., GANDHI P., FOELLMI C., GUTIERREZ C.M., LOPEZ-CORREDOIRA M.
	Astron. J., 137, 3263-3285 (2009)
	Multiwavelength study of the bright X-ray source population in the interacting galaxies NGC 5774/NGC 5775.
o	Table 1: <[GSG2009] NN> (Nos 1-49).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSG99]
[GSG99]	(Gaensler+Stappers+Getts, 1999)
Write:	<<[GSG99] JHHMMSS.s+DDMMSS.s>>
N:	1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Observation of an unresolved radio-source near the position of SAX J1808.4-3658. See also [RCM98], [SCM2000], [CSG2002b].
Ref:	=1999ApJ...522L.117G
by	GAENSLER B.M. , STAPPERS B.W., GETTS T.J.
	Astrophys. J., 522, 117-119 (1999)
	Transient radio emission from SAX J1808.4-3658.
o	<[GSG99] JHHMMSS.s+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GSGP
GSGP	(Gilmore, South Gal. Pole)= (SGP)
Write:	<<GSGP NN>>
Object:	* (SIMBAD class: Star)
Note:	Gilmore catalogue, described in 1982MNRAS.201...73R
Auth.:	GILMORE G.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: GSH
GSH	(Gal. Shell) (Not yet in Simbad)
*****	Avoid the usage of GSH, prefer [EP2013]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GSH
GSH	(Gal. Shell, Heiles)= (GS)
Write:	<<GSH LLL+BB+VVV>>
Object:	HI Shell (SIMBAD class: HIshell = Interstellar Shell)
Note:	First refs with Heiles Galactic Shells. In literature, 'GSH' shells are not always from Heiles.
Ref:	=1979ApJ...229..533H
by	HEILES C.
	Astrophys. J., 229, 533-544 (1979)
	H I shells and supershells.
o	Table 1: <GSH LLL+BB+VVV> N=63
Ref:	=1984ApJS...55..585H
by	HEILES C.
	Astrophys. J., Suppl. Ser., 55, 585-595 (1984)
	HI shells, supershells, shell-like objects, and "worms".
o	Table 1: <GSH LLL+BB+VVV> N=42
Ref:	=1989ApJ...336..808H
by	HEILES C.
	Astrophys. J., 336, 808-821 (1989)
	Magnetic fields, pressures and thermally unstable gas in prominent H I shells.
o	<GSH LLL+BB+VVV> N=4
Ref:	=1998ApJ...498..689H
by	HEILES C.
	Astrophys. J., 498, 689-703 (1998)
	Whence the Local Bubble, Gum, Orion? GSH 238+00+09, a nearby major superbubble toward galactic longitude 238°.
o	p.690 : GS 234-02 = part of [S87c] Loop 235-3
o	<GSH 238+00+09>
Ref:	=2002ApJ...578..176M
by	McCLURE-GRIFFITHS N.M. , DICKEY J.M., GAENSLER B.M., GREEN A.J.
	Astrophys. J., 578, 176-193 (2002)
	The galactic distribution of large H I shells.
o	Table 1: <GSH LLL+BB+VVV> N=15 added.
Ref:	=2005A&A...437..101E
by	EHLEROVA S. , PALOUS J.
	Astron. Astrophys., 437, 101-112 (2005)
	HI shells in the outer Milky Way.
o	Table 1: <GSH LLL+BB+VVV> N=628.
=E=	Catalogue in electronic form as J/A+A/437/101
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [GSH2006]
[GSH2006]	(Gossl+Snigula+Hopp, 2006)
Write:	<<[GSH2006] VNa>> <<[GSH2006] PN>>
N:	8+6
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Stat:	is completely incorporated in Simbad
Note:	Wendelstein 0.8m telescope observations. Search for Cepheids in Leo A and DDO 216 galaxies.
in source:	NAME Leo A
in source:	DDO 216
Ref:	=2006MmSAI..77..299G
by	GOESSL C.A. , SNIGULA J., HOPP U.
	Mem. Soc. Astron. Ital., 77, 299-302 (2006)
	Using δ Cep stars to study northern dwarf irregular galaxies of the Local Group.
o	Table 2: <[GSH2006] VNa> (Nos V1-V7, V6a), <[GSH2006] PN> (Nos P1-P6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GSHCTK
GSHCTK	(Grossschwabhausen Cassegrain Teleskop Kamera) (Not yet in Simbad)
Write:	<<GSHCTK JHHMMSS+DDMMSS>>
N:	about 100
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	In preparation. Project of deep imaging photometry in R and I band obtained with the CTK for a selected field in the Pleiades cluster. Several new Pleiades candidates but also new background sources are identified in a deep R and I band imaging. All those sources for which no accurate positions are listed in the 2MASS point source catalogue will be named with the new designation proposed here. Further new objects detected with the CTK in the future will get a similar designation.
in source:	NAME Pleiades
Auth.:	EISENBEISS T.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: GSI
GSI	(G, South, field I)
Write:	<<GSI NNN>>
N:	136
Object:	G (SIMBAD class: Galaxy)
Ref:	=1989MNRAS.236..207M
by	METCALFE N. , FONG R., SHANKS T., KILKENNY D.
	Mon. Not. R. Astron. Soc., 236, 207-234 (1989)
	An extended galaxy redshift survey - I. The catalogue.
o	<GNH NNN> (Nos 1-106), <GNX NNN> (Nos 1-113), <GNY NN> (Nos 1-91), <GNZ NNN> (Nos 1-130), <GSG NNN> (Nos 1-159), <GSI NNN> (Nos 1-136), <GSM NNN> (Nos 1-130), <GSN NNN> (Nos 1-195), <GSP NN> (Nos 1-74)
=E=	Catalogue in electronic form as J/MNRAS/236/207
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GSI2003]
[GSI2003]	(Gilbank+Smail+Ivison+, 2003)
Write:	<<[GSI2003] NNN>>
N:	224
Object:	Extremely Red Obj. (SIMBAD class: Galaxy)
Note:	NIR observations with INGRID at the William Herschel telescope (WHT). Use of archival HST data. Search for faint extremely red objects.
Ref:	=2003MNRAS.346.1125G
by	GILBANK D.G. , SMAIL I., IVISON R.J., PACKHAM C.
	Mon. Not. R. Astron. Soc., 346, 1125-1142 (2003)
	An HST morphological survey of faint extremely red objects.
o	Table 4: <[GSI2003] NNN> N=224 among (Nos 1-229).
=E=	Catalogue in electronic form as J/MNRAS/346/1125
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSI2007]
[GSI2007]	(Greve+Stern+Ivison+, 2007)
Write:	<<[GSI2007] MM JHHMMSS.s+DDMMSS>> <<[GSI2007] SMM JHHMMSS.s+DDMMSS>> <<[GSI2007] SMG JHHMMSS.s>> <<[GSI2007] MIPS N>>
N:	16
Object:	(mm) + G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	SHARC-II and MAMBO millimeter observations of the field of 4C 41.47. N=12 1200mu.m MAMBO sources, N=3 350mu.m SHARC-II sources, and N=14 Submillimeter selected Galaxies (SMG) + N=1 24mu.m source denoted MIPS 1 by the authors.
Ref:	=2007MNRAS.382...48G
by	GREVE T.R. , STERN D., IVISON R.J., DE BREUCK C., KOVACS A., BERTOLDI F.
	Mon. Not. R. Astron. Soc., 382, 48-66 (2007)
	Wide-field mid-infrared and millimetre imaging of the high-redshift radio galaxy, 4C41.17.
o	Fig.1, Table 1: <[GSI2007] MM JHHMMSS.s+DDMMSS> N=12, <[GSI2007] SMM JHHMMSS.s+DDMMSS> N=3. Fig.2, Tables 3, 4: <[GSI2007] SMG JHHMMSS.s> N=14, <[GSI2007] MIPS N> (No. 1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSJ2011]
[GSJ2011]	(Geers+Scholz+Jayawardhana+, 2011)
Write:	<<[GSJ2011] NN>>
N:	27
Object:	Poss. Brown Dwarf (SIMBAD class: BrownD*_Candidate = Brown Dwarf Candidate)
Stat:	is completely incorporated in Simbad
Note:	Subaru Suprime-Cam and MOIRCS observations of N=27 brown dwarf candidates in ρ Ophiuchi. Use of 2MASS and Spitzer data. See also [MSG2012], SONYC.
in source:	NAME rho Oph Cloud
Ref:	=2011ApJ...726...23G
by	GEERS V. , SCHOLZ A., JAYAWARDHANA R., LEE E., LAFRENIERE D., TAMURA M.
	Astrophys. J., 726, 23 (2011)
	Substellar objects in nearby young clusters (SONYC). II. The brown dwarf population of ρ Ophiuchi.
o	Table 1: <[GSJ2011] NN> (Nos 1-27). Table 2: <SONYC RhoOph-N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSK2002]
[GSK2002]	(Garcia-Ruiz+Sancisi+Kuijken, 2003)
Write:	<<[GSK2002] HHMMSS.s+DDMMSS>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=2 new companions of UGC 4806.
Ref:	=2002A&A...394..769G
by	GARCIA-RUIZ I. , SANCISI R., KUIJKEN K.
	Astron. Astrophys., 394, 769-789 (2002)
	Neutral hydrogen and optical observations of edge-on galaxies: Hunting for warps.
o	Table 7: <[GSK2002] HHMMSS.s+DDMMSS> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSK2010]
[GSK2010]	(Gouliermis+Schmeja+Klessen+, 2010)
Write:	<<[GSK2010] NN>>
N:	47
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Subaru SuprimeCam observations of N=47 distinct star clusters in NGC 6822.
in source:	NGC 6822
Ref:	=2010ApJ...725.1717G
by	GOULIERMIS D.A. , SCHMEJA S., KLESSEN R.S., DE BLOK W.J.G., WALTER F.
	Astrophys. J., 725, 1717-1734 (2010)
	Hierarchical stellar structures in the Local Group dwarf galaxy NGC 6822.
o	Tables 1, 3: <[GSK2010] NN> (Nos 1-47).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSL2002]
[GSL2002]	(Giveon+Sternberg+Lutz+, 2002)
Write:	<<[GSL2002] NNN>>
N:	149
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	ISO SWS observations of HII regions: (Nos 1-112) are galactic HII, (Nos 113-126) are in the LMC, (Nos 127-130) in the SMC, (Nos 131-149) are in M 33.
in source:	Magellanic Clouds:LMC = LMC
in source:	Magellanic Clouds:SMC = SMC
in source:	M 33 = NGC 598
Ref:	=2002ApJ...566..880G
by	GIVEON U. , STERNBERG A., LUTZ D., FEUCHTGRUBER H., PAULDRACH A.W.A.
	Astrophys. J., 566, 880-897 (2002)
	The excitation and metallicity of galactic H II regions from Infrared Space Observatory SWS observations of mid-infrared fine-structure lines.
o	(Erratum) Erratum vol. 575, p. 585 (2002)
o	Tables 2, 5, 6: <[GSL2002] NNN> (Nos 1-149).
=E=	Catalogue in electronic form as J/ApJ/566/880
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSL2004]
[GSL2004]	(Graham+Swift Li+, 2004)
Write:	<<[GSL2004] JHHMMSS.ss+DDMMSS.s>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	KAIT observations. Host G of SN 2004U and SN 2004V.
Ref:	=2004IAUC.8285....2G
by	GRAHAM J. , SWIFT B., LI W.
	IAU Circ., 8285, 2-None (2004)
	Supernovae 2004T, 2004U, and 2004V.
o	(Erratum) + corrigendum in IAUC 8286
o	Coordinates of SN 2004U and offset for SN 2004T : correct values in CBET 60.
o	<[GSL2004] JHHMMSS.ss+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSL2007]
[GSL2007]	(Grupe+Schady+Leighly+, 2007)
Write:	<<[GSL2007] Star N>>
N:	4
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Swift UVOT observations. Reference stars around the galaxy WPVS 7.
Ref:	=2007AJ....133.1988G
by	GRUPE D. , SCHADY P., LEIGHLY K.M., KOMOSSA S., O'BRIEN P.T., NOUSEK J.A.
	Astron. J., 133, 1988-1994 (2007)
	An update on the X-ray transient narrow-line Seyfert 1 galaxy WPVS 007: Swift observations of UV variability and persistence of X-ray faintness.
o	Table 4, Fig.3: <[GSL2007] Star N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSL2010]
[GSL2010]	(Gorlova+Steinhauser+Lada, 2010)
Write:	<<[GSL2010] NN>>
N:	30
Object:	Poss. YSO + * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	KPNO 2.1m and 4m telescopes FLAMINGOS observations of the Serpens Molecular Cloud.
in source:	NAME Serpens Cloud
Ref:	=2010ApJ...716..634G
by	GORLOVA N. , STEINHAUER A., LADA E.
	Astrophys. J., 716, 634-662 (2010)
	FLAMINGOS near infrared survey of the Serpens cloud main core.
o	Fig. 2, Tables 1-2: <[GSL2010] NN> (Nos 1-30).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSL98]
[GSL98]	(Gioia+Shaya+Le Fevre+, 1998)
Write:	<<[GSL98] A>> <<[GSL98] ANN>> <<[GSL98] N>>
N:	4+23+58
Object:	G + Arc (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	HST, ROSAT HRI and ASCA observations. Analysis of observations of the lensing cluster MS 0440+0204 = 1E 0440.5+0204 observed with different telescopes. Fig.2: N=4 galaxies, (Nos A-D), and N=23 arcs (Nos A1-A23). Fig.4, Table 1: Galaxies observed with the MMT, N=37, (Nos G1-G37). with the CFHT, N=4, (Nos C1-C4). with the Keck, N=9, (Nos K1-K9). and N=8 additional galaxies which are not cluster members, (Nos 1-8). See also [LGA93]
in source:	1E 0440.5+0204 = ClG 0440+02
Ref:	=1998ApJ...497..573G
by	GIOIA I.M. , SHAYA E.J., LE FEVRE O., FALCO E.E., LUPPINO G.A., HAMMER F.
	Astrophys. J., 497, 573-586 (1998)
	The lensing cluster MS 0440+0204 seen by HST, ROSAT, and ASCA. I. Cluster properties.
o	MS 0440+0204 = 1E 0440.5+0204. p.581 : MS 1512+3647 = 1E 1512.4+3647
o	Fig.2: <[GSL98] A> (Nos A-D), <[GSL98] ANN> (Nos A1-A23). Fig.4, Table 1: <[GSL98] ANN> (Nos G1-G37, C1-C4, K1-K9), <[GSL98] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GSM
GSM	(G, South, field M)
Write:	<<GSM NNN>>
N:	130
Object:	G (SIMBAD class: Galaxy)
Ref:	=1989MNRAS.236..207M
by	METCALFE N. , FONG R., SHANKS T., KILKENNY D.
	Mon. Not. R. Astron. Soc., 236, 207-234 (1989)
	An extended galaxy redshift survey - I. The catalogue.
o	<GNH NNN> (Nos 1-106), <GNX NNN> (Nos 1-113), <GNY NN> (Nos 1-91), <GNZ NNN> (Nos 1-130), <GSG NNN> (Nos 1-159), <GSI NNN> (Nos 1-136), <GSM NNN> (Nos 1-130), <GSN NNN> (Nos 1-195), <GSP NN> (Nos 1-74)
=E=	Catalogue in electronic form as J/MNRAS/236/207
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GSM2001]
[GSM2001]	(Gal-Yam+Sharon+Maoz, 2001)
Write:	<<[GSM2001] JHHMMSS.s+DDMMSS>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of SN 1996CP.
Ref:	=2001IAUC.7701....1G
by	GAL-YAM A. , SHARON K., MAOZ D.
	IAU Circ., 7701, 1-None (2001)
	Supernovae 1996cl, 1996cp, and 1996cq.
o	<[GSM2001] JHHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSM2009]
[GSM2009]	(Geach+Smail+Moran+, 2009)= (MIPS)
Write:	<<[GSM2009] MIPS JHHMMSS.s+DDMMSS.s>> <<[GSM2009] a>>
N:	12
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spitzer Infrared Spectrograph survey of 24mum selected luminous infrared galaxies in the rich cluster Cl 0024+16.
in source:	ClG 0024+1652 = HMS 0024+1654
Ref:	=2009ApJ...691..783G
by	GEACH J.E. , SMAIL I., MORAN S.M., TREU T., ELLIS R.S.
	Astrophys. J., 691, 783-793 (2009)
	The nature of dusty starburst galaxies in a rich cluster at z = 0.4: the progenitors of lenticulars?
o	Table 1: <[GSM2009] MIPS JHHMMSS.s+DDMMSS.s> N=12 = <[GSM2009] a> (Nos a-l).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSM2010]
[GSM2010]	(Guth+Shafter+Misselt, 2010)
Write:	<<[GSM2010] M94N YYYY-MMa>>
N:	4
Object:	Poss. Nova (SIMBAD class: Nova_Candidate = Classical Nova Candidate)
Stat:	is completely incorporated in Simbad
Note:	Steward Observatory 2.3m Bok telescope Halpha photometry of N=4 nova candidates in the early-type spiral galaxy M94.
in source:	NGC 4736 = M 94
Ref:	=2010ApJ...720.1155G
by	GUTH T. , SHAFTER A.W., MISSELT K.A.
	Astrophys. J., 720, 1155-1160 (2010)
	The nova rate in M94 (NGC 4736).
o	Table 2: <[GSM2010] M94N-YYYY-MMa> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GSN
GSN	(G, South, field N)
Write:	<<GSN NNN>>
N:	195
Object:	G (SIMBAD class: Galaxy)
Ref:	=1989MNRAS.236..207M
by	METCALFE N. , FONG R., SHANKS T., KILKENNY D.
	Mon. Not. R. Astron. Soc., 236, 207-234 (1989)
	An extended galaxy redshift survey - I. The catalogue.
o	<GNH NNN> (Nos 1-106), <GNX NNN> (Nos 1-113), <GNY NN> (Nos 1-91), <GNZ NNN> (Nos 1-130), <GSG NNN> (Nos 1-159), <GSI NNN> (Nos 1-136), <GSM NNN> (Nos 1-130), <GSN NNN> (Nos 1-195), <GSP NN> (Nos 1-74)
=E=	Catalogue in electronic form as J/MNRAS/236/207
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GSP
GSP	(G, South, field P)
Write:	<<GSP NN>>
N:	74
Object:	G (SIMBAD class: Galaxy)
Ref:	=1989MNRAS.236..207M
by	METCALFE N. , FONG R., SHANKS T., KILKENNY D.
	Mon. Not. R. Astron. Soc., 236, 207-234 (1989)
	An extended galaxy redshift survey - I. The catalogue.
o	<GNH NNN> (Nos 1-106), <GNX NNN> (Nos 1-113), <GNY NN> (Nos 1-91), <GNZ NNN> (Nos 1-130), <GSG NNN> (Nos 1-159), <GSI NNN> (Nos 1-136), <GSM NNN> (Nos 1-130), <GSN NNN> (Nos 1-195), <GSP NN> (Nos 1-74)
=E=	Catalogue in electronic form as J/MNRAS/236/207
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GSP2007]
[GSP2007]	(Gupta+Srianand+Petitjean+, 2007) (Not yet in Simbad)
Write:	<<[GSP2007] QSO JHHMM+DDMM abs N.NNNN>>
N:	10
Object:	Absorber
Note:	GMRT survey for 21cm absorbers from candidate DLA systems.
Ref:	=2007ApJ...654L.111G
by	GUPTA N. , SRIANAND R., PETITJEAN P., KHARE P., SAIKIA D.J., YORK D.G.
	Astrophys. J., 654L, 111-114 (2007)
	Detecting cold gas at intermediate redshifts: giant metrewave radio telescope survey using mg II systems.
o	Table 1: <[GSP2007] QSO JHHMM+DDMM abs N.NNNN> N=10.
Ref:	=2009MNRAS.398..201G
by	GUPTA N. , SRIANAND R., PETITJEAN P., NOTERDAEME P., SAIKIA D.J.
	Mon. Not. R. Astron. Soc., 398, 201-220 (2009)
	A complete sample of 21-cm absorbers at z ~ 1.3: Giant Metrewave Radio Telescope survey using Mg II systems.
o	Tables 2-3: <[GSP2007] QSO JHHMM+DDMM abs N.NNNN> N=25 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSP2013]
[GSP2013]	(Galametz+Stern+Pentericci+, 2013)
Write:	<<[GSP2013] NNNN>>
N:	45
Object:	G (SIMBAD class: Galaxy)
Note:	VLT FORS2 observations of N=48 galaxies in the field of the radio galaxy MRC 0156-252.
Ref:	=2013A&A...559A...2G
by	GALAMETZ A. , STERN D., PENTERICCI L., DE BREUCK C., VERNET J., WYLEZALEK D., FASSBENDER R., HATCH N., KURK J., OVERZIER R., RETTURA A., SEYMOUR N.
	Astron. Astrophys., 559A, 2-2 (2013)
	A large-scale galaxy structure at z=2.02 associated with the radio galaxy MRC 0156-252.
o	<NAME MRC 0156-252 Group> N=1. Table A.1-2: <[GSP2013] NNNN> N=10+35.
=E=	Catalogue in electronic form as <J/A+A/559/A2/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GSPC
GSPC	(Guide Star Photometric Catalog)
Write:	<<GSPC PNNN-A>> <<GSPC SNNN-A>>
N:	1477
Object:	Phe Std. * (SIMBAD class: Star)
Note:	All-sky set of 1477 photoelectrically determined BV sequences covering the magnitude range from 9 to 15. In the format, the first letter is 'P' for Palomar (Northern hemisphere) N=583, or 'S' for SERC (Southern hemisphere) N=894. Finding Charts.
Ref:	=1988ApJS...68....1L
by	LASKER B.M. , STURCH C.R., LOPEZ C., MALLAMA A.D., McLAUGHLIN S.F., RUSSELL J.L., WISNIEWSKI W.Z., GILLESPIE B.A., JENKNER H., SICILIANO E.D., KENNY D., BAUMERT J.H., GOLDBERG A.M., HENRY G.W., KEMPER E., SIEGEL M.J.
	Astrophys. J., Suppl. Ser., 68, 1-90 (1988)
	The guide star photometric catalog. I.
o	Updated Version 1 in 1996.
o	Table 7: <GSPC PNNN-A>, <GSPC SNNN-A>, N=1477
=E=	Catalogue in electronic form as II/143
Details on Acronym: GSPC2
GSPC2	(Guide Star Photometric Catalog, 2nd) (Not yet in Simbad)
Write:	<<GSPC2 ANNN-AAAA>>
N:	554007
Object:	Phe Std. * (SIMBAD class: Star)
Note:	Catalog of stars between 14-19th magnitude near the center of each of the Palomar and UKSTU survey fields.
Ref:	=2001A&A...368..335B
by	BUCCIARELLI B. , GARCIA YUS J., CASALEGNO R., POSTMAN M., LASKER B.M., STURCH C., LATTANZI M.G., McLEAN B.J., COSTA E., FALASCA A., LE POOLE R., MASSONE G., POTTER M., ROSENBERG A., BORGMAN T., DOGGETT J., MORRISON J., PIZZUTI A., POMPEI E., REHNER D., SICILIANO L., WOLFE D.
	Astron. Astrophys., 368, 335-346 (2001)
	An all-sky set of ((B)-V-R) photometric calibrators for Schmidt surveys. GSPC2.1: First release.
o	Catalog: <GSPC2 ANNN-AAAA> N=554007.
=E=	Catalogue in electronic form as II/272
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GSR2004]
[GSR2004]	(Gauinazzi+Siemiginowska+Rodriguez-Pascual+, 2004)
Write:	<<[GSR2004] JHHMMSS.s+DDMMSS>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton EPIC observations of Mkn 668. N=3 sources are detected within the field of Mkn 668.
in source:	Mrk 668
Ref:	=2004A&A...421..461G
by	GUAINAZZI M. , SIEMIGINOWSKA A., RODRIGUEZ-PASCUAL P., STANGHELLINI C.
	Astron. Astrophys., 421, 461-471 (2004)
	XMM-Newton discovery of a Compton-thick AGN in the GPS galaxy Mkn 668.
o	Table 1: <[GSR2004] JHHMMSS.s+DDMMSS> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSR2007]
[GSR2007]	(Geach Simpson+Rawlings, 2007)= (JEG) = (SXDF)
Write:	<<[GSR2007] JEGN>> <<[GSR2007] JEGN Group>> <<[GSR2007] SXDF-iE-NNNNNN>> <<[GSR2007] SXDF-iS-NNNNNN>>
N:	4+4+8+38
Object:	rG (SIMBAD class: RadioG = Radio Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Magellan 6.5m telescope LDSS spectroscopy of group of galaxies around radio galaxies in the SXDF field.
in source:	NAME SXDF
Ref:	=2007MNRAS.381.1369G
by	GEACH J.E. , SIMPSON C., RAWLINGS S., READ A.M., WATSON M.
	Mon. Not. R. Astron. Soc., 381, 1369-1380 (2007)
	Low-power radio galaxy environments in the Subaru/XMM-Newton Deep Field at z ~ 0.5.
o	Table 1: <[GSR2007] JEGN> (Nos JEG1 to JEG4). Text, Table 3:<[GSR2007] JEGN Group> (Nos JEG1 Group to JEG4 Group). Table 3: <[GSR2007] SXDF-iE-NNNNNN> N=8, <[GSR2007] SXDF-iS-NNNNNN> N=38.
=E=	Catalogue in electronic form as J/MNRAS/381/1369
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSR2015]
[GSR2015]	(Grillo+Suyu+Rosati+, 2015)
Write:	<<[GSR2015] GN>> <<[GSR2015] NN.N>> <<[GSR2015] s N>>
N:	2+30+3
Object:	G + Grav. lensed image of a G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Use of HST ACS and WFC3 data from the CLASH survey and of VLT VIMOS data from the CLASH-VLT survey in the field of the Frontier Fields galaxy cluster MCS J0416.0-2403 : N=2 brightest cluster galaxies, N=30 gravitationally lensed images (in ten systems), and N=3 other background sources.
in source:	MCS J0416.1-2403
Ref:	=2015ApJ...800...38G
by	GRILLO C. , SUYU S.H., ROSATI P., MERCURIO A., BALESTRA I., MUNARI E., NONINO M., CAMINHA G.B., LOMBARDI M., DE LUCIA G., BORGANI S., GOBAT R., BIVIANO A., GIRARDI M., UMETSU K., COE D., KOEKEMOER A.M., POSTMAN M., ZITRIN A., HALKOLA A., BROADHURST T., SARTORIS B., PRESOTTO V., ANNUNZIATELLA M., MAIER C., FRITZ A., VANZELLA E., FRYE B.
	Astrophys. J., 800, 38 (2015)
	CLASH-VLT: insights on the mass substructures in the frontier fields cluster MACS J0416.1-2403 through accurate strong lens modeling.
o	Fig. 1, Table 1: <[GSR2015] GN> (Nos G1-G2). Figs 1-2, Table 3: <[GSR2015] NN.N> (Nos 1.1-1.3 to 10.1-10.3). Fig. 3, Table 4: <[GSR2015] s N> (Nos s 1-s 3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GSS
GSS	(Groth Strip Survey)
*****	Avoid the usage of GSS, prefer [CHS2005]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GSS
GSS	(Groth Strip Survey)
*****	Avoid the usage of GSS, prefer DEEP-GSS
Origin	of the Acronym: L (2003ApJ...597..239G)
Details on Acronym: GSS
GSS	(Grasdalen+Strom+Strom)
Write:	<<GSS NN>>
N:	41
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Not numbered, but found numbered (format 'NN') in later literature. See the remark for VSSG.
in source:	NAME rho Oph Cloud
Ref:	=1973ApJ...184L..53G
by	GRASDALEN G.L. , STROM K.M., STROM S.E.
	Astrophys. J., 184, 53-57 (1973)
	A 2-micron map of the Ophiuchus dark-cloud region.
o	Table 2: S1 = GSS 35, S2 = GSS 32, S3 = GSS 6, S4 = GSS 8
o	Table 1: <GSS NN> (Nos 1-41), not numbered here. Table 2: <NAME SN IN RHO OPH CLOUD> (Nos S1-S4)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: GSS
GSS	(Grasdalen+Strom+Strom, 1973)
*****	Avoid the usage of GSS, prefer GSS
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GSS
GSS	(Groth Strip Survey)
*****	Avoid the usage of GSS, prefer [KVP96]
Origin	of the Acronym: L (2003ApJ...584...76C)
Details on Acronym: [GSS2005]
[GSS2005]	(Gupta+Srianand+Saikia, 2005)
Write:	<<[GSS2005] QSO J0137+3309 abs N.NNN>> <<[GSS2005] QSO J0137+3309 abs N.NNNN>>
N:	2
Object:	Absorber
Note:	HST STIS and GHRS, FUSE, and IUE observations. Detection of absorbers in the spectra of 3C 48 = QSO J0137+3309.
Ref:	=2005MNRAS.361..451G
by	GUPTA N. , SRIANAND R., SAIKIA D.J.
	Mon. Not. R. Astron. Soc., 361, 451-459 (2005)
	Outflowing material in the compact steep-spectrum source quasar 3C 48: evidence of jet-cloud interaction?
o	In chap. 4.1 : SBS 1542+531 is a misprint for SBS 1542+541.
o	Text: <[GSS2005] QSO J0137+3309 abs 0.3654>, <[GSS2005] QSO J0137+3309 abs 0.286>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSS2010]
[GSS2010]	(Galametz+Stern+Stanford+, 2010)
Write:	<<[GSS2010] Cl1756.NN>> <<[GSS2010] sBzK.NNNNN>> <<[GSS2010] pBzK.NNNNN>> <<[GSS2010] AGN.NNNN>> <<[GSS2010] 7C 1756+6520 cluster>>
N:	20+18+35+1
Object:	AGN + G + Cluster of G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck2 DEIMOS observations of galaxies in the vicinity of the radio galaxy 7C 1756+6520.
Ref:	=2010A&A...516A.101G
by	GALAMETZ A. , STERN D., STANFORD S.A., DE BREUCK C., VERNET J., GRIFFITH R.L., HARRISON F.A.
	Astron. Astrophys., 516A, 101-101 (2010)
	Spectroscopic confirmation of a galaxy cluster associated with 7C 1756+6520 at z=1.416.
o	Table 1, col(1): <[GSS2010] Cl1756.NN> (Nos 1-20). Tables 1-2, col(2): <[GSS2010] sBzK.NNNNN>, <[GSS2010] pBzK.NNNNN>, <[GSS2010] AGN.NNNN> N=18+35. Text: <[GSS2010] 7C 1756+6520 cluster> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSS95]
[GSS95]	(Giovanelli+Scodeggio+Solanes+, 1995)
Write:	<<[GSS95] A>>
N:	8
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Objects A, B, C, E and G are likely members of ACO 2634. Map Fig. 3.
in source:	ACO 2634
Ref:	=1995AJ....109.1451G
by	GIOVANELLI R. , SCODEGGIO M., SOLANES J.M., HAYNES M.P., ARCE H., SAKAI S.
	Astron. J., 109, 1451-1457 (1995)
	H I 2334+26: an extended H I cloud near Abell 2634.
o	Table 1 : galaxies with format 33NNNN are AGC.
o	<NAME HI 2334+26>, Table 1: <[GSS95] A> (Nos A-H)
Details on Acronym: [GSS99]
[GSS99]	(Grimberg+Sadler+Simkin, 1999)= ([GSS99a]) (Not yet in Simbad)
Write:	<<[GSS99] Knot A>> <<[GSS99] fN>> <<[GSS99] Region AN>>
N:	2+3+4
Object:	Feature (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Study of the rG PKS 0349-27: Fig.2: N=2 knots 'Knot A' and 'Knot B', and N=3 faint arcs 'f1' to 'f3'. Fig.3: N=4 regions 'AN',with A2 = Knot A and B1 = Knot B.
in source:	PKS 0349-27
Ref:	=1999ApJ...521..121G
by	GRIMBERG B.I. , SADLER E.M., SIMKIN S.M.
	Astrophys. J., 521, 121-133 (1999)
	Extended emission line gas in radio galaxies: PKS 0349-27.
o	Fig.2: <[GSS99] Knot A> (Nos A-B), <[GSS99] fN> (Nos f1-f3). Fig.3: <[GSS99] Region AN> (Nos A1-A2, B1-B2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSS99a]
[GSS99a]	(Grimberg+Sadler+Simkin, 1999) (Not yet in Simbad)
*****	Avoid the usage of [GSS99a], prefer [GSS99]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSS99b]
[GSS99b]	(Garnavich+Suntzeff+Schommer+, 1999)
Write:	<<[GSS99b] JHHMMSS.ss+DDMMSS.s>>
N:	13
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	CTIO Telescope observations. Host galaxies of SN 1999K to SN 1999W.
Ref:	=1999IAUC.7097Q...1G
by	GARNAVICH P. , SUNTZEFF N.B., SCHOMMER R.A., SMITH R.C., COVARRUBIAS R., SODERBERG A., CHALLIS P., SCHMIDT B., FILIPPENKO A.V., RIESS A.G., LEONARD D.C.
	IAU Circ., 7097, 1-None (1999)
	Supernovae.
o	<[GSS99b] JHHMMSS.ss+DDMMSS.s> N=13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GST2005]
[GST2005]	(Ghosh+Swartz+Tennant+, 2005)
Write:	<<[GST2005] N>>
N:	7
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra X-ray sources in NGC 5018.
in source:	NGC 5018
Ref:	=2005ApJ...623..815G
by	GHOSH K.K. , SWARTZ D.A., TENNANT A.F., WU K., SARIPALLI L.
	Astrophys. J., 623, 815-825 (2005)
	A multiwavelength study of the X-ray sources in NGC 5018.
o	Table 1: <[GST2005] N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GST2006]
[GST2006]	(Ganguly+Sembach+Tripp+, 2006)
Write:	<<[GST2006] QSO J0228-4057 abs N.NNNN>>
N:	1
Object:	Absorber
Note:	FUSE and HST STIS observations of QSO J0228-4057 = HE 0226-4110.
Ref:	=2006ApJ...645..868G
by	GANGULY R. , SEMBACH K.R., TRIPP T.M., SAVAGE B.D., WAKKER B.P.
	Astrophys. J., 645, 868-889 (2006)
	High-resolution absorption spectroscopy of multiphase, high-metallicity gas associated with the luminous quasar HE 0226-4110.
o	Text: <[GST2006] QSO J0228-4057 abs N.NNNN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GSW
GSW	(Gehrz+Sramek+Weedman)= ([GSW83])
Write:	<<GSW A>> <<GSW C'>> <<GSW a>> <<GSW ANN>> <<GSW C-Complex>> <<GSW C-East>> <<GSW C-West>> <<GSW C''>>
N:	58
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Sources and regions in the system NGC 3690+IC 694. Compact sources are indicated with capital letters 'A' and components 'AN' components B1 and B2 have sub-components B11-B17 and B21-B26 C+C' are forming the C-Complex. C1+C2 = C-West, C3 = C-East. Extended sources or regions are indicated with lowercase letters: Nos d-g. A Radio-source C" in the east of C' is found in 2003. Maps in each reference. See also [LRR99b].
in source:	NGC 3690
Ref:	=1983ApJ...267..551G
by	GEHRZ R.D. , SRAMEK R.A., WEEDMAN D.W.
	Astrophys. J., 267, 551-562 (1983)
	Star bursts and the extraordinary galaxy NGC 3690.
o	<GSW A> (Nos A-C), <GSW a> (Nos d-e), <GSW C'>.
Ref:	=1990ApJ...364...65B
by	BAAN W.A. , HASCHICK A.
	Astrophys. J., 364, 65-76 (1990)
	HI absorption and OH emission in IC 694/NGC 3690.
o	<GSW a> (Nos f-g), <GSW C-East>, <GSW C-West>, <GSW C-Complex> are new
Ref:	=1991ApJ...377..426W
by	WYNN-WILLIAMS C.G. , EALES S.A., BECKLIN E.E., HODAPP K.-W., JOSEPH R.D., McLEAN I.S., SIMONS D.A., WRIGHT G.S.
	Astrophys. J., 377, 426-433 (1991)
	Infrared emission regions in the interacting galaxy system Arp 299.
o	Fig.3: <GSW AN> (Nos B1-B2).
Ref:	=1997ApJ...475L.107A
by	AALTO S. , RADFORD S.J.E., SCOVILLE N.Z., SARGENT A.I.
	Astrophys. J., 475, 107-110 (1997)
	Variation of molecular line ratios and cloud properties in the Arp 299 galaxy merger.
o	<GSW AN> (Nos D, A1-A2, B3, C1-C3).
Ref:	=2000ApJ...532..845A
by	ALONSO-HERRERO A. , RIEKE G.H., RIEKE M.J., SCOVILLE N.Z.
	Astrophys. J., 532, 845-866 (2000)
	Extreme star formation in the interacting galaxy Arp 299 (IC 694+NGC 3690).
o	Fig.7, Table 4: <GSW AN> (Nos A3-A6, C4-C5, D1-D3) added, <GSW ANN> (Nos B11-B16, B21-B26).
Ref:	=2003ApJ...594L..31Z
by	ZEZAS A. , WARD M.J., MURRAY S.S.
	Astrophys. J., 594, 31-34 (2003)
	Chandra observations of the X-ray-luminous star-forming galaxy merger Arp 299.
o	Table 1: <[ZWM2003] NN> (Nos 1-18), <GSW C''> added.
Ref:	=2004ApJ...611..186N
by	NEFF S.G. , ULVESTAD J.S., TENG S.H.
	Astrophys. J., 611, 186-199 (2004)
	A supernova factory in the merger system Arp 299.
o	Text: <[NUT2004] JHHMMSS+DDMMSS> N=1. Fig.5, Table 7: <GSW AN> (No. A0) added.
Ref:	=2006ApJ...650..850G
by	GARCIA-MARIN M. , COLINA L., ARRIBAS S., ALONSO-HERRERO A., MEDIAVILLA E.
	Astrophys. J., 650, 850-871 (2006)
	Integral field spectroscopy of the luminous infrared galaxy Arp 299 (IC 694 + NGC 3690).
o	(Erratum) erratum vol. 654, p. 696 (2007)
o	Fig.1, Tables: <GSW ANN> (Nos F, G, H1-H2, I, I1, K1-K12) added.
Ref:	=2022A&A...658A...4R
by	RAMIREZ-OLIVENCIA N. , VARENIUS E., PEREZ-TORRES M., ALBERDI A., CONWAY J.E., ALONSO-HERRERO A., PEREIRA-SANTAELLA M., HERRERO-ILLANA R.
	Astron. Astrophys., 658A, 4-4 (2022)
	Sub-arcsecond LOFAR imaging of Arp 299 at 150 MHz. Tracing the nuclear and diffuse extended emission of a bright LIRG.
o	Fig.8, Paragr.4.4: <GSW ANN> (No. B17) added.
Origin	of the Acronym: L (1990ApJ...362..434C)
Details on Acronym: [GSW2003]
[GSW2003]	(Garnavich+Stanek+Wyrzykowski+, 2003) (Not yet in Simbad)
Write:	<<[GSW2003] A>>
N:	9
Object:	* (SIMBAD class: Star)
Note:	N=9 local standard stars in the field of GRB 011121.
Ref:	=2003ApJ...582..924G
by	GARNAVICH P.M. , STANEK K.Z., WYRZYKOWSKI L., INFANTE L., BENDEK E., BERSIER D., HOLLAND S.T., JHA S., MATHESON T., KIRSHNER R.P., KRISCIUNAS K., PHILLIPS M.M., CARLBERG R.G.
	Astrophys. J., 582, 924-932 (2003)
	Discovery of the low-redshift optical afterglow of GRB 011121 and its progenitor supernova SN 2001ke.
o	Table 1, Fig.1: <[GSW2003] A> (Nos A-I).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSW83]
[GSW83]	(Gehrz+Sramek+Weedman, 1983)
*****	Avoid the usage of [GSW83], prefer GSW
Origin	of the Acronym: S = Created by Simbad, the CDS Database
History	of this Acronym: replaced by GSW
Details on Acronym: [GSW97]
[GSW97]	(Greenhouse+Satyapal+Woodward+, 1997)
Write:	<<[GSW97] Fe N>>
N:	6
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=6 compact [Fe II] sources in M 82. Maps in Plates 1-2
in source:	M 82 = NGC 3034
Ref:	=1997ApJ...476..105G
by	GREENHOUSE M.A. , SATYAPAL S., WOODWARD C.E., FISCHER J., THOMPSON K.L., FORREST W.J., PIPHER J.L., RAINES N., SMITH H.A., WATSON D.M., RUDY R.J.
	Astrophys. J., 476, 105-112 (1997)
	Infrared Fabry-Perot imaging of M82 [Fe II] emission. II. Tracing extragalactic supernova remnants.
o	(Erratum) Erratum vol. 485, p. 438
o	Table 1: <[GSW97] Fe N> (Nos 1-6)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GSW98]
[GSW98]	(Greiner+Schwarz+Wenzel, 1998) (Not yet in Simbad)
Write:	<<[GSW98] Star A>>
N:	2
Object:	* (SIMBAD class: Star)
Note:	ROSAT All-SKy Survey. N=2 stars in the field of RX J1724.0+4114
Ref:	=1998MNRAS.296..437G
by	GREINER J. , SCHWARZ R., WENZEL W.
	Mon. Not. R. Astron. Soc., 296, 437-441 (1998)
	Discovery of the high-field polar RX J1724.0+4114.
o	Fig.2: <[GSW98] Star A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GSWC2003
GSWC2003	(Gomez+Stark+Whitney+Churchwell, 2003)
====>	Equivalent to: [GSWC2003]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GSWC2003]
[GSWC2003]	(Gomez+Stark+Whitney+Churchwell, 2003)= GSWC2003
Write:	<<[GSWC2003] NNaN>>
N:	70
Object:	H2 Knot (SIMBAD class: PartofCloud = Part of Cloud)
Note:	ESO NTT and WIYN observations. NIR 2.12 mu.m survey covering a large portion of the rho Ophiuchus cloud. Maps of H2 knots and components of knots.
in source:	NAME rho Oph Cloud
Ref:	=2003AJ....126..863G
by	GOMEZ M. , STARK D.P., WHITNEY B.A., CHURCHWELL E.
	Astron. J., 126, 863-886 (2003)
	Jets and Herbig-Haro objects in the ρ Ophiuchi embedded cluster.
o	Table 4: <[GSWC2003] NNaN> (Nos 1-26) N=68.
Ref:	=2006A&A...449.1077C
by	CARATTI O GARATTI A. , GIANNINI T., NISINI B., LORENZETTI D.
	Astron. Astrophys., 449, 1077-1088 (2006)
	H_{2} active jets in the near IR as a probe of protostellar evolution.
o	Fig.11, Table 7: <[DE95] NGC 2264G AN> (Nos I1-I5, H1-H5) added. Fig.12, Table 7: <[CGN2006] VLA 1623 A> (Nos A-D). Fig.12, Table 7: <[GSWC2003] NNa> (Nos 14h, 14i, 17b) added. Fig.17, Table 7: <[NMV2001] Knot A> (Nos N-R) added.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GSZ2000]
[GSZ2000]	(Greiner+Schwarz+Zharikov+, 2000)
Write:	<<[GSZ2000] A>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	(Nos A-B), two X-ray sources in the error circle of RX J1420.4+5334 observed by ROSAT.
Ref:	=2000A&A...362L..25G
by	GREINER J. , SCHWARZ R., ZHARIKOV S., ORIO M.
	Astron. Astrophys., 362, 25-28 (2000)
	RX J1420.4+5334 - another tidal disruption event?
o	Fig.3: <[GSZ2000] A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GT
GT	(Gregory+Taylor)
Write:	<<GT HHMM+DDda>>
N:	534+1274+20
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Format 'HHMM+DDd': truncated format. 1983AJ.....88.1784T: N=534 discrete radio-sources among which 15 variables sources newly discovered (Table V). 1988AJ.....95.1149D: 17 sources previously suspected variables are observed as variables.
Ref:	=1981ApJ...248..596G
by	GREGORY P.C. , TAYLOR A.R.
	Astrophys. J., 248, 596-605 (1981)
	Radio patrol of the Northern Milky Way: a survey for variable sources.
o	Table 3: <GT HHMM+DDd> N=5
Ref:	=1983AJ.....88.1784T
by	TAYLOR A.R. , GREGORY P.C.
	Astron. J., 88, 1784-1809 (1983)
	Radio patrol of the Northern Milky Way: a catalog of sources. I.
o	Table IV: <GT HHMM+DDda> N=534
Ref:	=1986AJ.....92..371G
by	GREGORY P.C. , TAYLOR A.R.
	Astron. J., 92, 371-411 (1986)
	Radio patrol of the Northern Milky Way: a catalog of sources. II.
o	Table II: <GT HHMM+DDda> N=1274
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GT89]
[GT89]	(Guhathakurta+Tyson, 1989)= (ir)
Write:	<<[GT89] irN>>
N:	4
Object:	(IR) (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Ref:	=1989ApJ...346..773G
by	GUHATHAKURTA P. , TYSON J.A.
	Astrophys. J., 346, 773-793 (1989)
	Optical characteristics of galactic 100 micron cirrus.
o	Table 1: <[GT89] irN> (Nos ir1 to ir4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTA2012]
[GTA2012]	(Goncalves+Teodorescu+Alves-Brito+, 2012)
Write:	<<[GTA2012] NN>>
N:	41
Object:	Poss. PN (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
Stat:	is completely incorporated in Simbad
Note:	Subaru FOCAS observations of N=41 PN candidates in IC10.
in source:	IC 10
Ref:	=2012MNRAS.425.2557G
by	GONCALVES D.R. , TEODORESCU A.M., ALVES-BRITO A., MENDEZ R.H., MAGRINI L.
	Mon. Not. R. Astron. Soc., 425, 2557-2566 (2012)
	A kinematic study of planetary nebulae in the dwarf irregular galaxy IC10.
o	Table 2: <[GTA2012] NN> (Nos 1-41).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTA99]
[GTA99]	(Giovannini+Taylor+Arbizzani+, 1999) (Not yet in Simbad)
Write:	<<[GTA99] A>> <<[GTA99] AN>> <<[GTA99] AAN>>
N:	4+7
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Fig.6: Southeast Jet of the rG B2 1144+35, N=1 Jet 'J' with 2 substructures 'J1' and 'J2', and N=1 counterjet 'CJ1'. Figs 13, 14: Image of the central source of B2 1144+35, N=7 components (Nos A-E, A1, B1). See also [SDR99].
in source:	B2 1144+35
Ref:	=1999ApJ...522..101G
by	GIOVANNINI G. , TAYLOR G.B., ARBIZZANI E., BONDI M., COTTON W.D., FERETTI L., LARA L., VENTURI T.
	Astrophys. J., 522, 101-112 (1999)
	B2 1144+35: a giant low-power radio galaxy with superluminal motion.
o	Fig.6: <[GTA99] J> N=1, <[GTA99] JN> (Nos J1-J2), <[GTA99] CJ1> N=1. Figs 13, 14: <[GTA99] AN> (Nos A-E, A1, B1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTC2005]
[GTC2005]	(Gonzalez+Tran+Conbere+, 2005)= (SG)
Write:	<<[GTC2005] N>> <<[GTC2005] SG JHHMM+DDMM>>
N:	6+1
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Chandra and optical spectroscopy observations: Detection of 6 X-ray detected galaxy groups, among which 3 referred to as a Super Group (SG).
Ref:	=2005ApJ...624L..73G
by	GONZALEZ A.H. , TRAN K.-V.H., CONBERE M.N., ZARITSKY D.
	Astrophys. J., 624, 73-76 (2005)
	Galaxy cluster assembly at z=0.37.
o	Table 1: <[GTC2005] N> (Nos 1-6). Text: <[GTC2005] SG J1120-1202> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTC2021]
[GTC2021]	(Garofalo+Tantalo+Cusano+, 2021)
Write:	<<[GTC2021] Pisces II VN>> <<[GTC2021] Pegasus III VN>>
N:	4+2
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	LBT LBC observations of N=4+2 variable stars in Milky Way ultra-faint dwarf satellite galaxies Pisces II and Pegasus III respectively.
in source:	NAME Psc II
in source:	NAME Peg III
Ref:	=2021ApJ...916...10G
by	GAROFALO A. , TANTALO M., CUSANO F., CLEMENTINI G., CALURA F., MURAVEVA T., PARIS D., SPEZIALI R.
	Astrophys. J., 916, 10-10 (2021)
	Born in a pair (?): Pisces II and Pegasus III.
o	Table 5: <[GTC2021] Pisces II VN> (Nos V1-V4), <[GTC2021] Pegasus III VN> (Nos V1-V2).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [GTD2001]
[GTD2001]	(Govoni+Taylor+Dallacasa+, 2001)
Write:	<<[GTD2001] AN>> <<[GTD2001] JHHMM+DDMM>>
N:	6
Object:	rG (SIMBAD class: RadioG = Radio Galaxy)
Stat:	is completely incorporated in Simbad
in source:	ACO 514
Ref:	=2001A&A...379..807G
by	GOVONI F. , TAYLOR G.B., DALLACASA D., FERETTI L., GIOVANNINI G.
	Astron. Astrophys., 379, 807-822 (2001)
	Radio galaxies and magnetic fields in A514.
o	Table 1: <[GTD2001] AN> (Nos A, B1-B2, C-E) = <[GTD2001] JHHMM+DDMM> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTE2015]
[GTE2015]	(Gouliermis+Thilker+Elmegreen+, 2015) (Not yet in Simbad)
Write:	<<[GTE2015] NNN>>
N:	244
Object:	Star Forming Region (SIMBAD class: StarFormingReg = Star Forming Region)
Note:	N=244 star-forming structures in NGC 6503. Use of HST LEGUS (Legacy ExtraGalactic UV Survey) photometry.
in source:	NGC 6503
Ref:	=2015MNRAS.452.3508G
by	GOULIERMIS D.A. , THILKER D., ELMEGREEN B.G., ELMEGREEN D.M., CALZETTI D., LEE J.C., ADAMO A., ALOISI A., CIGNONI M., COOK D.O., DALE D.A., GALLAGHER III J.S., GRASHA K., GREBEL E.K., DAVO A.H., HUNTER D.A., JOHNSON K.E., KIM H., NAIR P., NOTA A., PELLERIN A., RYON J., SABBI E., SACCHI E., SMITH L.J., TOSI M., UBEDA L., WHITMORE B.
	Mon. Not. R. Astron. Soc., 452, 3508-3528 (2015)
	Hierarchical star formation across the ring galaxy NGC 6503.
o	Table 2: <[GTE2015] NNN> (Nos 1-244).
=E=	Catalogue in electronic form as <J/MNRAS/452/3508/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTF2020]
[GTF2020]	(Gurri+Taylor+Fluke, 2020)
Write:	<<[GTF2020] IDNN>> <<[GTF2020] IDNN lens>> <<[GTF2020] IDNN system>>
N:	21
Object:	G + Grav. lens + Grav. lens system (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	ANU 2.3m telescope WiFeS observations of N=21 weakly lensed galaxies, along with N=21 gravitational lenses, forming N=21 gravitational lens systems.
Ref:	=2020MNRAS.499.4591G
by	GURRI P. , TAYLOR E.N., FLUKE C.J.
	Mon. Not. R. Astron. Soc., 499, 4591-4604 (2020)
	The first shear measurements from precision weak lensing.
o	Table 3: <[GTF2020] IDNN> (Nos ID1-ID21), <[GTF2020] IDNN lens> N=21, <[GTF2020] IDNN system> N=21.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTH2002]
[GTH2002]	(Greve+Tarchi+Huttemeister+, 2002)
Write:	<<[GTH2002] M-N>> <<[GTH2002] M-a>>
N:	6+4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	MERLIN observations. N=6 sources at 1.4 GHz in NGC 1569. N=4 tentative detection of point-like emission sources.
in source:	NGC 1569
Ref:	=2002A&A...381..825G
by	GREVE A. , TARCHI A., HUETTEMEISTER S., DE GRIJS R., VAN DER HULST J.M., GARRINGTON S.T., NEININGER N.
	Astron. Astrophys., 381, 825-833 (2002)
	A search for radio supernovae and supernova remnants in the region of NGC 1569's super star clusters.
o	In ref list, O'Connell, 1995: L10 is a misprint for L1 (1995ApJ...446L...1O). Objects cited as 'VLA-NN'are not in SIMBAD (van der Hulst+ in preparation, not published in 2008), but VLA-1 = [GTH2002] M-1, VLA-6 = [GTH2002] M-5, VLA-7 = [GTH2002] M-4, VLA-8 = EQ J043048.0+645056, VLA-10 = [GTH2002] M-2, VLA-11 = EQ J043045.7+645058, VLA-15 = [GTH2002] M-3, VLA-16 = EQ J043047.2+645104, VLA-19 = [GTH2002] M-1.
o	Table 2: <[GTH2002] M-N> (Nos M-1 to M-6). Table 3: <[GTH2002] M-a> (Nos M-a to M-d).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTJ2000]
[GTJ2000]	(Galadi-Enriquez+Trullols+Jordi, 2000)
Write:	<<[GTJ2000] FF-NNN>>
N:	681
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=681 secondary standard stars for CCD photometry, in 11 fields (Nos 1-11).
Ref:	=2000A&AS..146..169G
by	GALADI-ENRIQUEZ D. , TRULLOLS E., JORDI C.
	Astron. Astrophys., Suppl. Ser., 146, 169-177 (2000)
	Secondary UBVRI-CCD standard stars in the neighbourhood of Landolt standard stars.
o	Table 4: <[GTJ2000] FF-NNN> N=681.
=E=	Catalogue in electronic form as J/A+AS/146/169
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTJ84]
[GTJ84]	(Gavazzi+Tarenghi+Jaffe+, 1984)
Write:	<<[GTJ84] BHHMMSS+DDMMSS>> <<[GTJ84] ANN>>
N:	1+7+14
Object:	Feature (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=1 faint companion to UGC 6697, '114114+201515'. Brightest features in UGC 6697, (Nos A-F, R), but E and F seem to be not part of UGC. The features are sub-divided in knots 'AN', C12 being C1+C2 knots.
in source:	UGC 6697
Ref:	=1984A&A...137..235G
by	GAVAZZI G. , TARENGHI M., JAFFE W., BUTCHER H., BOKSENBERG A.
	Astron. Astrophys., 137, 235-244 (1984)
	Radio and optical investigation of UGC 6697 in Abell 1367.
o	Text, Fig.2: <[GTJ84] BHHMMSS+DDMMSS> N=1. Text, Fig.3: <[GTJ84] A> (Nos A-F, R). Text, Fig.7: <[GTJ84] AN> (Nos A1-A4, B1-B2, C1-C2, R1-R3).
Ref:	=1995A&A...304..325G
by	GAVAZZI G. , CONTURSI A., CARRASCO L., BOSELLI A., KENNICUTT R., SCODEGGIO M., JAFFE W.
	Astron. Astrophys., 304, 325-340 (1995)
	The radio and optical structure of three peculiar galaxies in A 1367.
o	Table 4, Fig.2a: <[GCC95] Z 97-73 A> (Nos A-D). Table 4, Fig.2b: <[GCC95] Z 97-79 A> (Nos A-E). Table 4, Fig.2c: <[GTJ84] AN> (No. B3) added.
Ref:	=2001A&A...377..745G
by	GAVAZZI G. , MARCELIN M., BOSELLI A., AMRAM P., VILCHEZ J.M., IGLESIAS-PARAMO J., TARENGHI M.
	Astron. Astrophys., 377, 745-758 (2001)
	The velocity field of UGC 6697 revisited.
o	Fig.1: <[GTJ84] AN> (No. R4) added. Table 6: <[GTJ84] ANN> (No. C12) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTK2008]
[GTK2008]	(Gavazzi+Treu+Koopmans+, 2008)
Write:	<<[GTK2008] Lens N>> <<[GTK2008] Source N>> <<[GTK2008] Ring N>>
N:	2+2+2
Object:	G + Grav. lensed image (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations of the lens system SDSS J094656.68+100652.8.
Ref:	=2008ApJ...677.1046G
by	GAVAZZI R. , TREU T., KOOPMANS L.V.E., BOLTON A.S., MOUSTAKAS L.A., BURLES S., MARSHALL P.J.
	Astrophys. J., 677, 1046-1059 (2008)
	The Sloan lens ACS survey. VI. Discovery and analysis of a double Einstein ring.
o	SDSS J0946+1006 = SDSS J094656.68+100652.8. Table 1: knots Na are not in SIMBAD.
o	Figs: <[GTK2008] Lens N> (Nos 1-2), <[GTK2008] Source N> (Nos 1-2), <[GTK2008] Ring N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTK91]
[GTK91]	(Georgiev+Tikhonov+Karachentsev+, 1991)
Write:	<<[GTK91] NNNA>> <<[GTK91] TNN>>
N:	110+70
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Format 'NNNA', (Nos 1-110, 17A, 23A). The stars (Nos 1-41) are identical to [S84b] Ho IX NN (Nos 1-41). Format 'TNN': secondary standard sequence stars, (Nos T1-T70).
in source:	Holmberg IX
in source:	M 81 = NGC 3031
Ref:	=1991A&AS...89..529G
by	GEORGIEV T.B. , TIKHONOV N.A., KARACHENTSEV I.D., BILKINA B.I.
	Astron. Astrophys., Suppl. Ser., 89, 529-536 (1991)
	The brightest stars and the distance to the dwarf galaxy Ho IX.
o	Table 1: <[GTK91] NNA> N=52. Table 2: <[GTK91] TNN> N=10
Ref:	=1992A&AS...96..569G
by	GEORGIEV T.B. , BILKINA B.I., TIKHONOV N.A.
	Astron. Astrophys., Suppl. Ser., 96, 569-581 (1992)
	The distribution of blue and red stars around the M 81 galaxy.
o	Kar 952+69 = DDO 66
o	Tables 2, 3: <[GTK91] TNN> (Nos T11-T70) added, <[GTK91] NNNA> (Nos 51-110) added. Table 4: <[GBT92] NE NN> (Nos 1-99). Table 5: <[GBT92] NW NN> (Nos 1-44). Table 6: <[GBT92] W NN> (Nos 1-76).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTK91b]
[GTK91b]	(Georgiev+Tikhonov+Karachentsev+, 1991)
Write:	<<[GTK91b] NN>>
N:	65
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Stat:	is completely incorporated in Simbad
Note:	see also [GTK91] and [GBT92]
in source:	M 81 = NGC 3031
Ref:	=1991PAZh...17..387G
by	GEORGIEV T.B. , TIKHONOV N.A., KARACHENTSEV I.D.
	Pis'ma Astron. Zh., 17, 387-392 (1991)
	The brightest globular candidates of M 81 galaxy.
o	translated in 1991SvAL.17.165G
o	<[GTK91b] NN> N=60
Ref:	=1993BSAO...36...43G
by	GEORGIEV T.B. , TIKHONOV N.A., BILKINA B.I., GETOV R.G., NEDIALKOV P.D.
	Bull. Special Astrophys. Obs., 36, 43-51 (1993)
	The precise coordinates of the supergiant and globular cluster candidates of the galaxy M81.
o	S = [S84b] M 81
o	Table 3: <[GTK91b] NN> (Nos 61-65) added
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTL2001]
[GTL2001]	(Grupe+Thomas+Leighly, 2001)
Write:	<<[GTL2001] N>> <<[GTL2001] A>>
N:	4+3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT observations of RX J2217.9-5941 field. Table 1: RASS sources (Nos 1-4). Table 2: ROSAT HRI sources (Nos A-C).
Ref:	=2001A&A...369..450G
by	GRUPE D. , THOMAS H.-C., LEIGHLY K.M.
	Astron. Astrophys., 369, 450-458 (2001)
	RX J2217.9-5941: A highly X-ray variable Narrow-Line Seyfert 1 galaxy.
o	Table 1: <[GTL2001] N> (Nos 1-4). Table 2: <[GTL2001] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTM2000]
[GTM2000]	(Gregory+Tifft+Moody+, 2000) (Not yet in Simbad)
Write:	<<[GTM2000] PFN>>
N:	3
Object:	Filament (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=3 'PF' (Perseus Filament).
in source:	NAME PER SUPERCL
Ref:	=2000AJ....119..567G
by	GREGORY S.A. , TIFFT W.G., MOODY J.W., NEWBERRY M.V., HALL S.M.
	Astron. J., 119, 567-572 (2000)
	The Arizona-New Mexico spectroscopic survey of galaxies. II. Structures in the Perseus supercluster.
o	Figs 1, 3: <[GTM2000] AAN> (Nos PF1-PF3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTM88]
[GTM88]	(Gregory+Tifft+Moody, 1988)
Write:	<<[GTM88] NN>>
N:	26
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
in source:	NAME Coma Supercluster
Ref:	=1988AJ.....95..662G
by	GREGORY S.A. , TIFFT W.G., MOODY J.W.
	Astron. J., 95, 662-667 (1988)
	Redshift studies of large-scale structure. II. A faint sample in the direction of the Coma/A 1367 supercluster.
o	Table I: <[GTM88] NN> (Nos 1-26)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTP2000]
[GTP2000]	(Gomez+Trapero+Pascual+, 2000)= (VLA)
Write:	<<[GTP2000] VLA BHHMM+DDd>>
N:	1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	N=1 unresolved source in the field of MBM 12, likely to be an extragalactic object.
Ref:	=2000MNRAS.314..743G
by	GOMEZ J.F. , TRAPERO J., PASCUAL S., PATEL N., MORALES C., TORRELLES J.M.
	Mon. Not. R. Astron. Soc., 314, 743-746 (2000)
	Ammonia observations of the nearby molecular cloud MBM 12.
o	p.744: <[GTP2000] VLA B0253+192> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTR2007]
[GTR2007]	(Grutzbauch+Trinchieri+Rampazzo+, 2007)
Write:	<<[GTR2007] RR NNN NNNNN>> <<[GTR2007] RR NNN X NN>>
N:	151+174+163+102+40+43
Object:	* + X (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	XMM-Newton observations and ESO 2.2m WFI telescope photometry of RR95 galaxy pairs.
in source:	RR95 143
in source:	RR95 210
in source:	RR95 216
in source:	RR95 242
Ref:	=2007AJ....133..220G
by	GRUETZBAUCH R. , TRINCHIERI G., RAMPAZZO R., HELD E.V., RIZZI L., SULENTIC J.W., ZEILINGER W.W.
	Astron. J., 133, 220-254 (2007)
	Small-scale systems of galaxies. III. X-ray-detected Elliptical+Spiral galaxy pairs in low-density environments.
o	Table 5: <[GTR2007] RR 143 NNNNN> N=151 among (Nos 6-25500). Table 6: <[GTR2007] RR 210 NNNNN> N=174 among (Nos 129-18444). Table 7: <[GTR2007] RR 216 NNNNN> N=163 among (Nos 15-24410). Table 8: <[GTR2007] RR 242 NNNNN> N=102 among (Nos 17-38663). Table 9: <[GTR2007] RR 143 X NN> (Nos 1-40). Table 10: <[GTR2007] RR 242 X NN> (Nos 1-43).
=E=	Catalogue in electronic form as J/AJ/133/220
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTS2010]
[GTS2010]	(Grant+Taylor+Stil+, 2010)= (DRAO)
Write:	<<[GTS2010] DRAO JHHMMSS.ss+DDMMSS.ss>>
N:	136
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Deep polarization imaging of the ELAIS N1 field at 1.4GHz with the Dominion Radio Astrophysical Observatory
in source:	ELAIS N1
Ref:	=2010ApJ...714.1689G
by	GRANT J.K. , TAYLOR A.R., STIL J.M., LANDECKER T.L., KOTHES R., RANSOM R.R., SCOTT D.
	Astrophys. J., 714, 1689-1701 (2010)
	The DRAO planck deep fields: the polarization properties of radio galaxies at 1.4 GHz.
o	Table 1: <[GTS2010] DRAO JHHMMSS.ss+DDMMSS.ss> N=136.
=E=	Catalogue in electronic form as J/ApJ/714/1689
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTT2004]
[GTT2004]	(Glazebrook+Tober+Thomson+, 2004)
Write:	<<[GTT2004] NNN>>
N:	8
Object:	G (SIMBAD class: Galaxy)
Note:	Results of a survey of the HDFN using Taurus Tunable Filter at the William Herschel Telescope. 8 galaxies are found from a synthetic catalogue of 351 possible objects.
in source:	NAME HDFN
Ref:	=2004AJ....128.2652G
by	GLAZEBROOK K. , TOBER J., THOMSON S., BLAND-HAWTHORN J., ABRAHAM R.
	Astron. J., 128, 2652-2659 (2004)
	Cosmic star formation history to z=1 from a narrow emission line-selected tunable-filter survey.
o	Table 2: <[GTT2004] NNN> N=8 among 351.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GTV2000]
[GTV2000]	(Galama+Tanvir+Vreeswijk+, 2000)
Write:	<<[GTV2000] A>>
N:	8
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=8 reference stars in the field of GRB 970228.
Ref:	=2000ApJ...536..185G
by	GALAMA T.J. , TANVIR N., VREESWIJK P.M., WIJERS R.A.M.J., GROOT P.J., ROL E., VAN PARADIJS J., KOUVELIOTOU C., FRUCHTER A.S., MASETTI N., PEDERSEN H., MARGON B., DEUTSCH E.W., METZGER M., ARMUS L., KLOSE S., STECKLUM B.
	Astrophys. J., 536, 185-194 (2000)
	Evidence for a supernova in reanalyzed optical and near-infrared images of GRB 970228.
o	Host Galaxy not identified, could be [ZSB98] G1 or [ZSB98] G3.
o	Table 2: <[GTV2000] A> (Nos A-H).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GUB2008]
[GUB2008]	(Groenewegen+Udalsi+Bono, 2008)
Write:	<<[GUB2008] bulNNN.N NNNNNN>>
N:	10
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Stat:	is completely incorporated in Simbad
Note:	NTT SOFI observations of cepheids in the Galactic Center identified in the OGLE database.
in source:	NAME Gal Center
Ref:	=2008A&A...481..441G
by	GROENEWEGEN M.A.T. , UDALSKI A., BONO G.
	Astron. Astrophys., 481, 441-448 (2008)
	The distance to the Galactic centre based on Population II Cepheids and RR Lyrae stars.
o	Table 1: Objects bulNN NNNNNN = OGLEII DIA BUL-SCNN NNNNNN in SIMBAD.
o	Table 1: <[GUB2008] bulNNN.N NNNNNN> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GUL2013]
[GUL2013]	(Glikman+Urrutia+Lacy+, 2013)
Write:	<<[GUL2013] JHHMMSS.ss+DDMMSS.s>> <<[GUL2013] UKFS HHMM+DDMM>>
N:	87+14
Object:	Red QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Note:	Palomar Hale telescope TripleSpec observations of N=87 reddened quasar candidates in FIRST and UKIDSS. Use of archival SDSS data.
Ref:	=2013ApJ...778..127G
by	GLIKMAN E. , URRUTIA T., LACY M., DJORGOVSKI S.G., URRY M., CROOM S., SCHNEIDER D.P., MAHABAL A., GRAHAM M., GE J.
	Astrophys. J., 778, 127 (2013)
	Dust reddened quasars in FIRST and UKIDSS: beyond the tip of the iceberg.
o	Table 1: <[GUL2013] JHHMMSS.ss+DDMMSS.s> N=87, Table 2: <[GUL2013] UKFS HHMM+DDMM> N=14.
=E=	Catalogue in electronic form as J/ApJ/778/127
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Gulliver
Gulliver	(Gulliver)
Write:	<<Cl Gulliver NN>>
N:	60
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	N=60 Galactic star clusters identification based on the DR2 Gaia data release.
Ref:	=2018A&A...618A..93C
by	CANTAT-GAUDIN T. , JORDI C., VALLENARI A., BRAGAGLIA A., BALAGUER-NUNEZ L., SOUBIRAN C., BOSSINI D., MOITINHO A., CASTRO-GINARD A., KRONE-MARTINS A., CASAMIQUELA L., SORDO R., CARRERA R.
	Astron. Astrophys., 618A, 93-93 (2018)
	A Gaia DR2 view of the open cluster population in the Milky Way.
o	Table 1: <Cl Gulliver NN> (Nos 1-60).
=E=	Catalogue in electronic form as J/A+A/618/A93
Origin	of the Acronym: A = Assigned by the author(s)
History	of this Acronym: replaces [CJV2018]
Details on Acronym: Gum
Gum	(Gum)= (G) = (Str) = (Stromlo)
Write:	<<Gum NNa>> <<Gum NN>>
N:	98
Object:	HII (4PN) (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	PN -> Gum 27, 47, 52, 60
Ref:	=1955MmRAS..67..155G
by	GUM C.S.
	Mem. R. Astron. Soc., 67, 155-177 (1955)
	A survey of southern HII regions.
o	Table I: <Gum NNa> (Nos 1-85) N=98.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Gunn
Gunn	(Gunn)
Write:	<<Gunn Ton 256B>> <<Gunn PKS 2251+11 N>> <<Gunn PKS 2251+11 Wisp>>
N:	1+7+1
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 1: 'Ton 256B is a companion of Ton 256. Fig.1: (Nos 1-7) objects in the field of PKS 2251+11 and W = Wisp.
Ref:	=1971ApJ...164L.113G
by	GUNN J.E.
	Astrophys. J., 164, 113-118 (1971)
	On the distances of the Quasi-Stellar Objects.
o	Table 1: <Gunn Ton 256B> N=1. Fig.1: <Gunn PKS 2251+11 N> (Nos 1-7), <Gunn PKS 2251+11 Wisp> N=1.
Origin	of the Acronym: L (1999A&AS..135...83M)
Details on Acronym: [GUS98]
[GUS98]	(Golap+Udaya Shankar+Sachdev+, 1998) (Not yet in Simbad)
Write:	<<[GUS98] JHHMMSS+DDMM>>
N:	25
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1998JApA...19...35G
by	GOLAP K. , UDAYA SHANKAR N., SACHDEV S., DODSON R., SASTRY C.V.
	J. Astrophys. Astron., 19, 35-53 (1998)
	A low frequency radio telescope at Mauritius for a southern sky survey.
o	Initial results, Table 3 not in SIMBAD.
o	Table 3: <[GUS98] JHHMMSS-DDMM> N=25.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GUSBAD
GUSBAD	(Gamma-ray bursts Uniformly Selected from Batse Archival Data)
Write:	<<GUSBAD YYMMDD.ddd>>
N:	2204
Object:	(Gamma) (SIMBAD class: gammaBurst = Gamma-ray Burst)
Note:	The GUSBAD catalog is based on BATSE DISCLA data for the full Compton Gamma Ray Observatory mission from April 19, 1991 till May 26, 2000. The GUSBAD catalog is uniform in the sense that the detection criterion is the same throughout and that the properties given in the catalog are available for every burst. Since the detection and derivation of properties listed in the catalog were carried out automatically (with rare exceptions), the catalog is especially suitable for statistical work and simulations, such as used in the evaluation of V/Vmax. http://www.astro.caltech.edu/~mxs/grb/GUSBAD/
Ref:	=2004ApJ...616.1072S
by	SCHMIDT M.
	Astrophys. J., 616, 1072-1077 (2004)
	The GUSBAD catalog of γ-ray bursts.
o	Catalog: <GUSBAD YYMMDD.ddd> N=2204.
=E=	Catalogue in electronic form as J/ApJ/616/1072
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: GUVV
GUVV	(GALEX UV Variability catalog)
Write:	<<GUVV JHHMMSS.s+DDMMSS.s>>
N:	44+410
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Note:	Galaxy Evolution Explorer (GALEX) UV Variability catalog contains information on 84 sources gained with Near and Far UV photometric observations.
Ref:	=2005AJ....130..825W
by	WELSH B.Y. , WHEATLEY J.M., HEAFIELD K., SEIBERT M., BROWNE S.E., SALIM S., RICH R.M., BARLOW T.A., BIANCHI L., BYUN Y.-I., DONAS J., FORSTER K., FRIEDMAN P.G., HECKMAN T.M., JELINSKY P.N., LEE Y.-W., MADORE B.F., MALINA R.F., MARTIN D.C., MILLIARD B., MORRISSEY P., NEFF S.G., SCHIMINOVICH D., SIEGMUND O.H.W., SMALL T., SZALAY A.S., WYDER T.K.
	Astron. J., 130, 825-831 (2005)
	The GALEX ultraviolet variability catalog.
o	Table 2: <GUVV JHHMMSS.s+DDMMSS.s> N=44.
Ref:	=2008AJ....136..259W
by	WHEATLEY J.M. , WELSH B.Y., BROWNE S.E.
	Astron. J., 136, 259-266 (2008)
	The second GALEX ultraviolet variability (GUVV-2) catalog.
o	Table 2: <GUVV JHHMMSS.s+DDMMSS.s> N=410.
=E=	Catalogue in electronic form as J/AJ/130/825
=E=	Catalogue in electronic form as <J/AJ/136/259/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GV
GV	(Grande Vitesse)= (F) = (FD) = (G)
Write:	<<GV NNN>> <<GV NNNbis>> <<GV NNNter>>
N:	767
Object:	* (SIMBAD class: Star)
Note:	Identif. charts. Also 1972A&A vol. 16 p.365-444, and 1982A&AS...48....1F. Revision is given in 1982A&AS...48..409F. 1982A&AS...48..409F: also contains 711 stars [FD82] NNN. cross-id. that revise and complete 1974A&AS...13..173F. additional G numbers (ex. G 225ter, G 234bis). See also PV and [FD70]
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1970A&ASS...1....1F
by	FEHRENBACH C. , DUFLOT M.
	Astron. Astrophys., Special Suppl. Ser., 1, 1-67 (1970)
	Grand Nuage de Magellan. Liste des etoiles membres du Grand Nuage de Magellan et liste d'etoiles galactiques.
o	<GV NNN> (Nos 1-495). <PV NNNN> (Nos 1-1830). <[FD70] SNNN> (Nos S1-S110).
Ref:	=1973A&AS...10..231F
by	FEHRENBACH C. , DUFLOT M.
	Astron. Astrophys., Suppl. Ser., 10, 231-265 (1973)
	Grand nuage de Magellan. Seconde liste d'etoiles membres du grand nuage de Magellan et liste d'etoiles galactiques.
o	<GV NNN> (Nos 501-588), <PV NNNN> (Nos 2001-2253)
Ref:	=1981A&AS...46...13F
by	FEHRENBACH C. , DUFLOT M., DUFLOT A., GENTY V., MANNONE C.
	Astron. Astrophys., Suppl. Ser., 46, 13-19 (1981)
	Grand Nuage de Magellan. Troisieme liste d'etoiles membres du Grand Nuage de Magellan et liste d'etoiles galactiques.
o	<GV NNN> (Nos 601-767), <PV NNNN> (Nos 2501-2990)
Ref:	=1982A&AS...48..409F
by	FEHRENBACH C. , DUFLOT M.
	Astron. Astrophys., Suppl. Ser., 48, 409-442 (1982)
	Vitesses radiales au prisme objectif dans la direction du Grand Nuage de Magellan.
o	revision of <GV NNN> and <PV NNNN>. New numbering for GV list: <[FD82] NNN> (Nos 1-711).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GV
GV	(Grueff+Vigotti)
*****	Avoid the usage of GV, prefer [GV68]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [GV2003]
[GV2003]	(Gvaramadze+Vikhlinin, 2003)
Write:	<<[GV2003] W>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of SNR 315.4-2.3. N=2 X-ray point sources.
in source:	SNR G315.4-02.3
Ref:	=2003A&A...401..625G
by	GVARAMADZE V.V. , VIKHLININ A.A.
	Astron. Astrophys., 401, 625-630 (2003)
	Point X-ray sources in the SNR G315.4-2.30 (MSH 14-63, RCW 86).
o	Fig.2: <[GV2003] W> (Nos N, S).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GV2007]
[GV2007]	(Girart+Viti, 2007)
Write:	<<[GV2007] N>>
N:	5
Object:	HH (SIMBAD class: HerbigHaroObj = Herbig-Haro Object)
Stat:	is completely incorporated in Simbad
Note:	SEST observations of the molecular environment ahead of HH 188.
Ref:	=2007A&A...470..633G
by	GIRART J.M. , VITI S.
	Astron. Astrophys., 470, 633-638 (2007)
	The origin of the molecular emission around the southern hemisphere Re 4 IRS - HH 188 region.
o	Table 3: <[GV2007] N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GV2009]
[GV2009]	(Giacintucci+Venturi, 2009)
Write:	<<[GV2009] GMRT JHHMM+DDMM>>
N:	4
Object:	rG (SIMBAD class: RadioG = Radio Galaxy)
Stat:	is completely incorporated in Simbad
Note:	GMRT 610MHz and 327MHz observations of N=4 radio galaxies with tailed morphology.
Ref:	=2009A&A...505...55G
by	GIACINTUCCI S. , VENTURI T.
	Astron. Astrophys., 505, 55-61 (2009)
	Tailed radio galaxies as tracers of galaxy clusters. Serendipitous discoveries with the GMRT.
o	Table 1: <[GV2009] GMRT JHHMM+DDMM> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GV68]
[GV68]	(Grueff+Vigotti, 1968)= (GV)
Write:	<<[GV68] NNN>>
N:	328
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1968ApL.....2..113G
by	GRUEFF G. , VIGOTTI M.
	Astrophys. Lett., 2, 113-120 (1968)
	A pencil-beam deep sky survey at 408 MHz.
o	Table I: <[GV68] NNN> (Nos 1-328)
Details on Acronym: [GV72]
[GV72]	(Grueff+Vigotti, 1972)
Write:	<<[GV72] HHMM+DDA>>
N:	19
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Tables 1, 2: Among the 265+223 radio-sources, 19 are not in the B2 catalog.
Ref:	=1972A&AS....6....1G
by	GRUEFF G. , VIGOTTI M.
	Astron. Astrophys., Suppl. Ser., 6, 1-84 (1972)
	Optical identification of radio-sources selected from the B2 catalogue.
o	Tables 1, 2: Among the 265+223 radio sources, 19 are not in the B2 catalog, they are designated as '[GV72] HHMM+DDA' in SIMBAD. Table 3: reference stars are not in SIMBAD.
o	Tables 1, 2: <[GV72] HHMM+DDA> N=19.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVA2004]
[GVA2004]	(Gerssen+Van der Marel+Axon+, 2004)
Write:	<<[GVA2004] NGC 6240 AN>> <<[GVA2004] NGC 6240 AN'>> <<[GVA2004] JHHMMSS.sss+DDMMSS.ss>>
N:	4+1
Object:	Nucleus + * (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 and NICMOS study of the morphology of NGC 6240. Three nuclear regions are found, region N1 has a sourthern extension designated N1'. An uncataloged star is found in the map 'J165259.847+022412.60'.
in source:	NGC 6240
Ref:	=2004AJ....127...75G
by	GERSSEN J. , VAN DER MAREL R.P., AXON D., MIHOS J.C., HERNQUIST L., BARNES J.E.
	Astron. J., 127, 75-89 (2004)
	Hubble space telescope observations of NGC 6240: a case study of an ultraluminous infrared galaxy with obscured activity.
o	Fig.3, Table 2: <[GVA2004] NGC 6240 AN> (Nos N1-N3), <[GVA2004] NGC 6240 AN'> (No. N1'). Text: <[GVA2004] JHHMMSS.sss+DDMMSS.ss> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVB2004]
[GVB2004]	(Giacintucci+Venturi+Bardelli+, 2004)
Write:	<<[GVB2004] JHHMM+DDMMa>>
N:	174
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA 1.4GHz observations of the region between the centres of ACO 3558 and ACO 3562.
in source:	NAME ACO 3558 Complex
Ref:	=2004A&A...419...71G
by	GIACINTUCCI S. , VENTURI T., BARDELLI S., DALLACASA D., ZUCCA E.
	Astron. Astrophys., 419, 71-87 (2004)
	AGN and starburst radio activity in the A3558 cluster complex.
o	Table 3: Designation '# NNNNN' from Yentis+ 1992 not in SIMBAD.
o	Table 3: <[GVB2004] JHHMM+DDMMa> N=174.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVB2006]
[GVB2006]	(Giacintucci+Venturi+Bardelli+, 2006)= (GMRT) = ([GVB2006a])
Write:	<<[GVB2006] JHHMM+DDMMa>> <<[GVB2006] J0454-1017a A>>
N:	52+3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Radio observations of ACO 521 with the GMRT (Giant Metrewave Radio Telescope). N =52 radio sources are found. In the radio relic, 3 radio galaxies are embedded (Nos A-C).
in source:	ACO 521
Ref:	=2006NewA...11..437G
by	GIACINTUCCI S. , VENTURI T., BARDELLI S., BRUNETTI G., CASSANO R., DALLACASA D.
	New Astronomy, 11, 437-451 (2006)
	The cluster relic source in A 521.
o	The cluster relic source = [GVB2006] J0454-1017a in SIMBAD. Optical identification MBP is a misprint for MPB ([MPB2000] in SIMBAD).
o	Table 3: <[GVB2006] JHHMM+DDMMa> N=52. Fig.5, text: <[GVB2006] J0454-1017a A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVB2006a]
[GVB2006a]	(Giacintucci+Venturi+Bardelli+, 2006)
*****	Avoid the usage of [GVB2006a], prefer [GVB2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVB2006b]
[GVB2006b]	(Glazebrook+Verma+Boyle+, 2006)
Write:	<<[GVB2006b] phot NNNN>> <<[GVB2006b] slit NNN>>
N:	5632
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	AAT imaging and LDSS observations. Deep photometric catalogue and associated spectroscopic redshift survey in the vicinity of the HDFS.
in source:	NAME HDFS
Ref:	=2006AJ....131.2383G
by	GLAZEBROOK K. , VERMA A., BOYLE B., OLIVER S., MANN R.G., MONBLEAU D.
	Astron. J., 131, 2383-2393 (2006)
	Anglo-Australian Telescope imaging and microslit spectroscopy in the southern Hubble Deep Field.
o	Table 1: <[GVB2006b] phot NNNN> (Nos 1-5632). Table 2: <[GVB2006b] slit NNN> (Nos 1-225).
=E=	Catalogue in electronic form as J/AJ/131/2383
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVB2009]
[GVB2009]	(Giacintucci+Venturi+Brunetti+, 2009) (Not yet in Simbad)
Write:	<<[GVB2009] A>> <<[GVB2009] PN>> <<[GVB2009] Clump W>>
N:	8+2+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA 1.4GHz and GMRT 240MHz observations of the giant radio halo in RXC J2003.5-2323.
Ref:	=2009A&A...505...45G
by	GIACINTUCCI S. , VENTURI T., BRUNETTI G., DALLACASA D., MAZZOTTA P., CASSANO R., BARDELLI S., ZUCCA E.
	Astron. Astrophys., 505, 45-53 (2009)
	Testing the radio halo-cluster merger scenario. The case of RXC J2003.5-2323.
o	Fig. 1: <[GVB2009] A> (Nos A-H). Fig. 5: <[GVB2009] PN> (Nos P1-P2), <[GVB2009] Clump W> (Nos Clump N, Clump S).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVC2009]
[GVC2009]	(Giacintucci+Venturi+Cassano+, 2009) (Not yet in Simbad)
Write:	<<[GVC2009] A>>
N:	7
Object:	rG (SIMBAD class: RadioG = Radio Galaxy)
Note:	Use of archival VLA data at 1.4GHz to optically identify N=7 radio galaxies in ACO 1351.
in source:	ACO 1351
Ref:	=2009ApJ...704L..54G
by	GIACINTUCCI S. , VENTURI T., CASSANO R., DALLACASA D., BRUNETTI G.
	Astrophys. J., 704L, 54-57 (2009)
	A giant radio halo in the massive and merging cluster Abell 1351.
o	Fig. 1: <[GVC2009] A> (Nos A-G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVC73]
[GVC73]	(Giovanelli+Verschuur+Cram, 1973)= (A) = (C) = (M)
Write:	<<[GVC73] A R.N>> <<[GVC73] C R A>> <<[GVC73] M R.N>>
N:	9+4+6
Object:	Concentration (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	λ - 21 cm. HPBW = 9'.7. Concentrations in complex [H68] A (format A R.N), in complex [H68] C (format C R A) (see also[W2001c], in complex [H68] M (format M R.N). Also studies concentrations in 0MM360 and HVC 112+2-139. See also [H68], HVC and IVC. See also [SSH76], [SO81], [WS91].
in source:	[H68] A
in source:	[H68] C
in source:	[H68] M
Ref:	=1973A&AS...12..209G
by	GIOVANELLI R. , VERSCHUUR G.L., CRAM T.R.
	Astron. Astrophys., Suppl. Ser., 12, 209-262 (1973)
	High resolution studies of high velocity clouds of neutral hydrogen.
o	Table 8: concentration in OMM 360 (=Ohio MM 360) not in SIMBAD
o	Table 3: <[H68] A R> N=6 (Nos A I to A VI). Table 4: <[GVC73] A R.N> N=9 (Nos A I.1 to A I.4, A II.1 to AII.2, A IV.1 to A IV.3). Table 5, Fig.8: <[GVC73] C R A> N=4 (Nos C I B, C III A to C III C). Table 7: <[GVC73] M R.N> N=6 (Nos I.1 to M I.3, M II.1 to M II.3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVD2017]
[GVD2017]	(Golovich+van Weeren+Dawson+, 2017)
Write:	<<[GVD2017] JDDD.dddddd+DD.ddddd>> <<[GVD2017] ZwCl 0008+5215 W>>
N:	202+2
Object:	G + Subcluster of G (SIMBAD class: Galaxy)
Note:	Keck II DEIMOS, Subaru SuprimeCam, HST ACS and WFC3, Chandra ACIS-I, and JVLA observations of N=202 galaxies in the field of the galaxy cluster ZwCl 0008+5215 and of N=2 subclusters of galaxies.
in source:	ZwCl 0008+5215
Ref:	=2017ApJ...838..110G
by	GOLOVICH N. , VAN WEEREN R.J., DAWSON W.A., JEE M.J., WITTMAN D.
	Astrophys. J., 838, 110-110 (2017)
	MC2: multiwavelength and dynamical analysis of the merging galaxy cluster ZwCl 0008.8+5215: an older and less massive Bullet Cluster.
o	Table 2: <[GVD2017] JDDD.dddddd+DD.ddddd> N=202. Fig. 1: <[GVD2017] ZwCl 0008+5215 W> (Nos E, W).
=E=	Catalogue in electronic form as <J/ApJ/838/110/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVD92]
[GVD92]	(Gregorini+Vettolani+De Ruiter+, 1992)
Write:	<<[GVD92] HHMMSS.s+DDMMSS>>
N:	85
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Ref:	=1992A&AS...95....1G
by	GREGORINI L. , VETTOLANI G., DE RUITER H.R., PARMA P.
	Astron. Astrophys., Suppl. Ser., 95, 1-7 (1992)
	Samples of dumb-bell galaxies in southern rich clusters.
o	Tables 1, 2, 3, 4: <[GVD92] HHMMSS.s-DDMMSS> N=85
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVG2006]
[GVG2006]	(Gawiser+van Dokkum+Gronwall+, 2006)
Write:	<<[GVG2006] BVR NNNNN>> <<[GVG2006] NB NNNNN>>
N:	84410+28297
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Broadband and deep narrowband photometry of the Extended Chandra Deep Field-South, as part of the MUSYC survey. In the formats, BVR means combined B+V+R images were used, and NB means that a NB5000 narrow-band image was used.
in source:	NAME ECDFS
Ref:	=2006ApJ...642L..13G
by	GAWISER E. , VAN DOKKUM P.G., GRONWALL C., CIARDULLO R., BLANC G.A., CASTANDER F.J., FELDMEIER J., FRANCKE H., FRANX M., HABERZETTL L., HERRERA D., HICKEY T., INFANTE L., LIRA P., MAZA J., QUADRI R., RICHARDSON A., SCHAWINSKI K., SCHIRMER M., TAYLOR E.N., TREISTER E., URRY C.M., VIRANI S.N.
	Astrophys. J., 642, 13-16 (2006)
	The physical nature of Lyα-emitting galaxies at z=3.1.
o	BVRdet: <[GVG2006] BVR NNNNN> (Nos 0-84409). NBdet: <[GVG2006] NB NNNNN> (Nos 0-28296).
=E=	Catalogue in electronic form as <J/ApJ/642/L13/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVG2010]
[GVG2010]	(Geha+van der Marel+Guhathakurta+, 2010)
Write:	<<[GVG2010] NGC NNN NNN>>
N:	520+442
Object:	RGB* (SIMBAD class: RGB* = Red Giant Branch star)
Stat:	is completely incorporated in Simbad
Note:	Keck II DEIMOS observations of NGC 147 and NGC 185.
in source:	NGC 147
in source:	NGC 185
Ref:	=2010ApJ...711..361G
by	GEHA M. , VAN DER MAREL R.P., GUHATHAKURTA P., GILBERT K.M., KALIRAI J., KIRBY E.N.
	Astrophys. J., 711, 361-373 (2010)
	Local Group dwarf elliptical galaxies. II. Stellar kinematics to large radii in NGC 147 and NGC 185.
o	Table 6: <[GVG2010] NGC 147 NNN> (Nos 1-520). Table 7: <[GVG2010] NGC 185 NNN> (Nos 1-442).
=E=	Catalogue in electronic form as J/ApJ/711/361
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVG2013]
[GVG2013]	(Giovannini+Vacca+Girardi+, 2013)
Write:	<<[GVG2013] Northern peak>>
N:	1
Object:	Poss. Cluster of G (SIMBAD class: ClG_Candidate = Cluster of Galaxies Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=1 galaxy overdensity to the north of ACO 3411. Use of data from the SuperCOSMOS Science Archive.
Ref:	=2013MNRAS.435..518G
by	GIOVANNINI G. , VACCA V., GIRARDI M., FERETTI L., GOVONI F., MURGIA M.
	Mon. Not. R. Astron. Soc., 435, 518-523 (2013)
	The nature of the giant diffuse non-thermal source in the A3411-A3412 complex.
o	Table 1: <[GVG2013] Northern peak> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVH2006]
[GVH2006]	(Gawiser+Van Dokkum+Herrera+, 2006)
Write:	<<[GVH2006] NNNNN>>
N:	62968
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Photometric catalogue of objects taken with MOSAIC on the CTIO 4m telescope of the extended HDFS, one of the field of the MUSYC survey.
in source:	NAME HDFS
Ref:	=2006ApJS..162....1G
by	GAWISER E. , VAN DOKKUM P.G., HERRERA D., MAZA J., CASTANDER F.J., INFANTE L., LIRA P., QUADRI R., TONER R., TREISTER E., URRY C.M., ALTMANN M., ASSEF R., CHRISTLEIN D., COPPI P.S., DURAN M.F., FRANX M., GALAZ G., HUERTA L., LIU C., LOPEZ S., MENDEZ R., MOORE D.C., RUBIO M., RUIZ M.T., TOFT S., YI S.K.
	Astrophys. J., Suppl. Ser., 162, 1-19 (2006)
	The Multiwavelength Survey by Yale-Chile (MUSYC): survey design and deep public UBVRIz' images and catalogs of the Extended Hubble Deep Field-South.
o	Table 7, col(1): <[GVH2006] NNNNN> (Nos 0-62967) = Table 7, col(2): <MUSYC JHHMMSS.ss+DDMMSS.s> N=62968.
=E=	Catalogue in electronic form as J/ApJS/162/1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVL2012]
[GVL2012]	(Gratton+Villanova+Lucatello+, 2012)
Write:	<<[GVL2012] ANN>> <<[GVL2012] ASNN>>
N:	81 (SIMBAD class: Star)
Note:	VLT FLAMES GIRAFFE spectrocopy of N=18+30+15+18 subgiant branch stars in NGC 1851. Use of archival HST data.
in source:	NGC 1851
Ref:	=2012A&A...544A..12G
by	GRATTON R.G. , VILLANOVA S., LUCATELLO S., SOLLIMA A., GEISLER D., CARRETTA E., CASSISI S., BRAGAGLIA A.
	Astron. Astrophys., 544A, 12-12 (2012)
	Spectroscopic analysis of the two subgiant branches of the globular cluster NGC 1851.
o	Table 1: <[GVL2012] ANN> N=18 among (Nos A03 to A35), <[GVL2012] A§NN> N=29 among (Nos AS05 to AS56). Table 2: <[GVL2012] ANN> N=15 among (Nos B01 to B18), <[GVL2012] A§NN> N=15 among (Nos BS03 to BS21)
Ref:	=2014MNRAS.442.3044M
by	MARINO A.F. , MILONE A.P., YONG D., DOTTER A., DA COSTA G., ASPLUND M., JERJEN H., MacKEY D., NORRIS J., CASSISI S., SBORDONE L., STETSON P.B., WEISS A., APARICIO A., BEDIN L.R., LIND K., MONELLI M., PIOTTO G., ANGELONI R., BUONANNO R.
	Mon. Not. R. Astron. Soc., 442, 3044-3064 (2014)
	The halo+cluster system of the Galactic globular cluster NGC 1851.
o	Tables 2-3: <[MMY2014] newNN> N=16 among (Nos 56 to 93), <[MMY2014] TNNN> N=94 among (Nos 048 to 222), <[GVL2012] ASNN> (Nos AS57, BS24, BS26, BS29) added.
=E=	Catalogue in electronic form as <J/MNRAS/442/3044/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVM2007]
[GVM2007]	(Giacintucci+Venturi+Murgia+, 2007) (Not yet in Simbad)
Write:	<<[GVM2007] A NNNN A>> <<[GVM2007] A NNNN AA>> <<[GVM2007] MKW N A>> <<[GVM2007] MKW Ns A>> <<[GVM2007] AWM N A>>
N:	29
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	GMRT observations of radio morphology of galaxy clusters.
in source:	ACO 1663
in source:	ACO 1775
in source:	ACO 2372
in source:	ACO 2622
in source:	AWM 5
in source:	MKW 1
in source:	MKW 2
in source:	MKW 6
in source:	MKW 7
in source:	MKW 3s
Ref:	=2007A&A...476...99G
by	GIACINTUCCI S. , VENTURI T., MURGIA M., DALLACASA D., ATHREYA R., BARDELLI S., MAZZOTTA P., SAIKIA D.J.
	Astron. Astrophys., 476, 99-119 (2007)
	Radio morphology and spectral analysis of cD galaxies in rich and poor galaxy clusters.
o	Radio in Tables 3 to 5 are not in SIMBAD.
o	Figs 1 to 11, Tables 3, 4, 5: <[GVM2007] A NNNN A>, <[GVM2007] A NNNN AA>, <[GVM2007] MKW N A>, <[GVM2007] MKW Ns A>, <[GVM2007] AWM N A>, N=29.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVM97]
[GVM97]	(Greiner+Van Paradijs+Marshall+, 1997)
Write:	<<[GVM97] RN>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations: N=3 X-ray sources in the RXTE (Rossi X-ray Timing Explorer) error box of GRB 970616. See also [HKM97].
Ref:	=1997IAUC.6722R...1G
by	GREINER J. , VAN PARADIJS J., MARSHALL F.M., HURLEY K., ROBINSON C., SIEBERT J.
	IAU Circ., 6722, 1-None (1997)
	GRB 970616.
o	Numbering 'RN' for the 3 ROSAT sources is found in 1999A&AS..138..455G
o	<[GVM97] RN> (Nos R1-R3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVR2012]
[GVR2012]	(Gomez+Valkonen+Romer+, 2012)
Write:	<<[GVR2012] NNNN>>
N:	116
Object:	G (SIMBAD class: Galaxy)
Note:	Gemini GMOS observations of N=116 galaxies in the field of the galaxy cluster ACO S 1063.
in source:	ACO S 1063
Ref:	=2012AJ....144...79G
by	GOMEZ P.L. , VALKONEN L.E., ROMER A.K., LLOYD-DAVIES E., VERDUGO T., CANTALUPO C.M., DAUB M.D., GOLDSTEIN J.H., KUO C.L., LANGE A.E., LUEKER M., HOLZAPFEL W.L., PETERSON J.B., RUHL J., RUNYAN M.C., REICHARDT C.L., SABIRLI K.
	Astron. J., 144, 79 (2012)
	Optical and X-ray observations of the merging cluster AS1063.
o	Table 2: <[GVR2012] NNNN> N=116 among (Nos 67-2000).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVR97]
[GVR97]	(Ghisellini+Villata+Riteri+, 1997)
Write:	<<[GVR97] S5 0716+714 A>>
N:	4
Object:	* (SIMBAD class: Star)
Note:	N=4 reference stars in the field of S5 0716+714. Finding chart.
Ref:	=1997A&A...327...61G
by	GHISELLINI G. , VILLATA M., RAITERI C.M., BOSIO S., DE FRANCESCO G., LATINI G., MAESANO M., MASSARO E., MONTAGNI F., NESCI R., TOSTI G., FIORUCCI M., PIAN E., MARASCHI L., TREVES A., COMASTRI A., MIGNOLI M.
	Astron. Astrophys., 327, 61-71 (1997)
	Optical-IUE observations of the γ-ray loud BL Lacertae object S5 0716+714: data and interpretation.
o	Table 1: <[GVR97] S5 0716+714 A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVS2000]
[GVS2000]	(Goedhart+Van der Walt+Schutte, 2000)
Write:	<<[GVS2000] HHMMm+DDMMA>>
N:	73
Object:	CH3OH Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	N=56 CH3OH masers towards IRAS sources. A letter 'A' at the end of the format indicates that multiple sources were found in the IRAS error box. See also [SVG93], [VGM95].
Ref:	=2000MNRAS.315..316G
by	GOEDHART S. , VAN DER WALT D.J., SCHUTTE A.J.
	Mon. Not. R. Astron. Soc., 315, 316-324 (2000)
	Infrared emission from 6.7-GHz methanol maser sources.
o	p.320 IRAS 1911-1048 (G45.07+0.13) misprint for IRAS 19110+1045 ?
o	Table 1: <[GVS2000] HHMMm+DDMMA> N=73.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVS2003]
[GVS2003]	(Garnavich+Von Braun+Stanek, 2003)
Write:	<<[GVS2003] Star A>>
N:	2
Object:	* (SIMBAD class: Star)
Note:	Stars in the field of GRB 030226. See also [PSA2004].
Ref:	=2003GCN..1885....1G
by	GARNAVICH P. , VON BRAUN K., STANEK K.
	GRB Coordinates Network, Circular Service, 1885, 1-None (2003)
	GRB 030226, optical observations.
o	<[GVS2003] Star A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVS98]
[GVS98]	(Gim+Vandenberg+Stetson+, 1998)
Write:	<<[GVS98] NNNNN>>
N:	15617
Object:	* (SIMBAD class: Star)
Note:	1.8m Plaskett Telescope at the Dominion Astrophysical Observatory (DAO) photometry of N=15617 stars within 18' of the center of NGC 7789.
in source:	NGC 7789
Ref:	=1998PASP..110.1318G
by	GIM M. , VANDENBERG D.A., STETSON P.B., HESSER J.E., ZUREK D.R.
	Publ. Astron. Soc. Pac., 110, 1318-1335 (1998)
	The open cluster NGC 7789. II. CCD VI photometry.
o	Table 5, col(3): <Cl* NGC 7789 G NNNN> N=44. table.dat: <[GVS98] NNNNN> (Nos 1-15617).
=E=	Catalogue in electronic form as J/PASP/110/1318
Details on Acronym: [GVV98]
[GVV98]	(Galama+Vreeswijk+Van Paradijs+, 1998)
Write:	<<[GVV98] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=1 unusual variable radio-source in the error box of GRB 981220. See also [CG98].
Ref:	=1998GCN...168....1G
by	GALAMA T.J. , VREESWIJK P., VAN PARADIJS J., KOUVELIOTOU C., STROM R., DE BRUYN G.
	GRB Coordinates Network, Circular Service, 168, 1-None (1998)
	GRB 981220, radio observations.
o	<[GVV98] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GVW2012]
[GVW2012]	(Greve+Vieira+Weiss+, 2012)
Write:	<<[GVW2012] SPT-S JHHMMSS+DDMM.m A>> <<[GVW2012] SPT-S JHHMMSS+DDMM.m-A>> (not recognised by Simbad, but found in literature) <<[GVW2012] SPT-S HHMM+DDA>>
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	APEX LABOCA and SABOCA 870µm and 350µm observations of SPT-S sources.
in source:	SPT-S J233227-5358.0
in source:	SPT-S J234942-5638.0
Ref:	=2012ApJ...756..101G
by	GREVE T.R. , VIEIRA J.D., WEISS A., AGUIRRE J.E., AIRD K.A., ASHBY M.L.N., BENSON B.A., BLEEM L.E., BRADFORD C.M., BRODWIN M., CARLSTROM J.E., CHANG C.L., CHAPMAN S.C., CRAWFORD T.M., DE BREUCK C., DE HAAN T., DOBBS M.A., DOWNES T., FASSNACHT C.D., FAZIO G., GEORGE E.M., GLADDERS M., GONZALEZ A.H., HALVERSON N.W., HEZAVEH Y., HIGH F.W., HOLDER G.P., HOLZAPFEL W.L., HOOVER S., HRUBES J.D., JOHNSON M., KEISLER R., KNOX L., LEE A.T., LEITCH E.M., LUEKER M., LUONG-VAN D., MALKAN M., MARRONE D.P., McINTYRE V., McMAHON J.J., MEHL J., MENTEN K.M., MEYER S.S., MONTROY T., MURPHY E.J., NATOLI T., PADIN S., PLAGGE T., PRYKE C., REICHARDT C.L., REST A., ROSENMAN M., RUEL J., RUHL J.E., SCHAFFER K.K., SHARON K., SHAW L., SHIROKOFF E., STALDER B., STANFORD S.A., STANISZEWSKI Z., STARK A.A., STORY K., VANDERLINDE K., WALSH W., WELIKALA N., WILLIAMSON R.
	Astrophys. J., 756, 101 (2012)
	Submillimeter observations of millimeter bright galaxies discovered by the South Pole Telescope.
o	Fig. 1, Table 1: <[GVW2012] SPT-S JHHMMSS+DDMM.m-A> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GW
GW	(Gravitational Wave) (Not yet in Simbad)
====>	Equivalent to: GrW
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GW
GW	(Gal. Worm)
Write:	<<GW LLL.l+B.b>>
N:	118
Object:	Gal. Worm (SIMBAD class: HI = HI (21cm) Source)
Note:	Table 2 : N=118, The running number in col(1) is not used. The worms correspond to the 'HI worms' detected by Heiles. HI, 60µm and 100µm features perpendicular to the gal. plane, might be debris of superbubbles. Finding charts.
Ref:	=1992ApJ...390..108K
by	KOO B.-C. , HEILES C., REACH W.T.
	Astrophys. J., 390, 108-132 (1992)
	Galactic worms. I. Catalog of worm candidates.
o	Table 2, col(2): <GW LLL.l+B.b> N=118.
=E=	Catalogue in electronic form as <J/ApJ/390/108/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GW2008]
[GW2008]	(Gendre+Wall, 2008)
Write:	<<[GW2008] CoNFIG NNN>> <<[GW2008] CoNFIG-N JHHMMSS.ss+DDMMSS.ss>> <<[GW2008] CoNFIG N-NNN>>
N:	859
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	The Combined NVSS-FIRST Galaxies (CoNFIG) samples. The CoNFIG sample is constructed as a sample of N=859 radio sources from NVSS with S≥1.3Jy. The CoNFIG-2, 3 and 4 samples are complete to 0.8Jy, 0.2Jy and 50mJy respectively.
Ref:	=2008MNRAS.390..819G
by	GENDRE M.A. , WALL J.V.
	Mon. Not. R. Astron. Soc., 390, 819-828 (2008)
	The Combined NVSS-FIRST Galaxies (CoNFIG) sample - I. Sample definition, classification and evolution.
o	(Erratum) erratum vol. 394, p. 1712 (2009)
o	Table A: <[GW2008] CoNFIG NNN> N=274 among (Nos 1-277). Table B1: <[GW2008] CoNFIG-2 JHHMMSS.ss+DDMMSS.ss> N=243. Table B2: <[GW2008] CoNFIG-3 JHHMMSS.ss+DDMMSS.ss> N=291, <[GW2008] CoNFIG-4 JHHMMSS.ss+DDMMSS.ss> N=234.
Ref:	=2010MNRAS.404.1719G
by	GENDRE M.A. , BEST P.N., WALL J.V.
	Mon. Not. R. Astron. Soc., 404, 1719-1732 (2010)
	The combined NVSS-FIRST galaxies (CoNFIG) sample - II. Comparison of space densities in the Fanaroff-Riley dichotomy.
o	Tables config[1-4].dat: <[GW2008] CoNFIG N-NNN> (Nos 1-1 to 1-274, 2-1 to 2-243, 3-1 to 3-287, 4-1 to 4-188) = <[GW2008] CoNFIG-N JHHMMSS.ss+DDMMSS.ss> N=859.
=E=	Catalogue in electronic form as J/MNRAS/390/819
=E=	Catalogue in electronic form as J/MNRAS/404/1719
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GW2022]
[GW2022]	(Ge+Wang, 2022)
Write:	<<[GW2022] FNNN>>
N:	163
Object:	Filament (SIMBAD class: Filament = Interstellar Filament)
Note:	N=163 large-scale filaments in the inner Galactic plane (\|l\|<60° with \|b\|<1.5°) from ATLASGAL clumps. Use of ATLASGAL data.
Ref:	=2022ApJS..259...36G
by	GE Y. , WANG K.
	Astrophys. J., Suppl. Ser., 259, 36-36 (2022)
	A Census of 163 Large-scale (>=10 pc), Velocity-coherent Filaments in the Inner Galactic Plane: Physical Properties, Dense-gas Fraction, and Association with Spiral Arms.
o	Figs D1-D2, Table 1: <[GW2022] FNNN> (Nos F1-F163).
=E=	Catalogue in electronic form as <J/ApJS/259/36/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [GW94]
[GW94]	(Goldader+Wynn-Williams, 1994)= (RS)
Write:	<<[GW94] NN>>
N:	16
Object:	Red * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	W 51
Ref:	=1994ApJ...433..164G
by	GOLDADER J.D. , WYNN-WILLIAMS C.G.
	Astrophys. J., 433, 164-178 (1994)
	Near-infrared observations of W 51.
o	Table 1, Fig.4: <[WBN74] W 51 IRS N> (No. 3). Table 1: <[GW94] NN> (Nos 1-16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GW98]
[GW98]	(Gregg+West, 1998)
Write:	<<[GW98] N>>
N:	4
Object:	Feature (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Kitt Peak Burrell Schmidt 0.6m telescope optical observations of the inner 3x3 degrees of the Coma cluster.
in source:	Coma Cluster = ACO 1656
Ref:	=1998Natur.396..549G
by	GREGG M.D. , WEST M.J.
	Nature, 396, 549-552 (1998)
	Galaxy disruption as the origin of intracluster light in the Coma cluster of galaxies.
o	Fig.1: <[GW98] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWA2003]
[GWA2003]	(Gao+Wang+Appleton+, 2003)
Write:	<<[GWA2003] NN>>
N:	31
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra-ACIS detection of ultraluminous sources in the Cartwheel galaxy system.
in source:	NAME Cartwheel Galaxy
Ref:	=2003ApJ...596L.171G
by	GAO Y. , WANG Q.D., APPLETON P.N., LUCAS R.A.
	Astrophys. J., 596, 171-174 (2003)
	Nonnuclear hyper/ultraluminous X-ray sources in the starbursting Cartwheel ring galaxy.
o	Table 1: <[GWA2003] NN> (Nos 1-31).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWA94]
[GWA94]	(Greene+Wilking+Andre+, 1994)
*****	Avoid the usage of [GWA94], prefer GWAYL
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GWAC
GWAC	(Ground-based Wide Angle Camera)
Write:	<<GWAC YYMMDDA>>
Object:	Opt. Transient (SIMBAD class: Transient = Transient Event)
Note:	The main science objective of the Ground-based Wide Angle Camera (GWAC) is to observe in the visible range (between 500 and 850nm) from the ground, the prompt emission of some of the gamma-ray bursts detected by SVOM camera ECLAIRs.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: GWAYL
GWAYL	(Greene+Wilking+Andre+Young+Lada)= ([GWA94]) = (IRS)
Write:	<<GWAYL N>>
N:	7
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=7 infrared sources in the nearby LDN 1689 and LDN 1709 clouds.
in source:	NAME RHO OPH CLOUD:LDN 1689 = LDN 1689
in source:	NAME RHO OPH CLOUD:LDN 1709 = LDN 1709
Ref:	=1994ApJ...434..614G
by	GREENE T.P. , WILKING B.A., ANDRE P., YOUNG E.T., LADA C.J.
	Astrophys. J., 434, 614-626 (1994)
	Further mid-infrared study of the ρ Ophiuchi cloud young stellar population : luminosities and masses of pre-main-sequence stars.
o	Table 1: <GWAYL N> (Nos 1-7)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWB2000]
[GWB2000]	(Gregg+Wisotzki+Becker+, 2000)
Write:	<<[GWB2000] 0512-3329 A>> <<[GWB2000] Star N>>
N:	2+9
Object:	Component + * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST STIS observations. N=2 components of the lensed QSO 0512-3329, (Nos A-B). N=9 stars in the field of the QSO. See also [WWL2003].
in source:	QSO B0512-3329
Ref:	=2000AJ....119.2535G
by	GREGG M.D. , WISOTZKI L., BECKER R.H., MAZA J., SCHECHTER P.L., WHITE R.L., BROTHERTON M.S., WINN J.N.
	Astron. J., 119, 2535-2539 (2000)
	A close-separation double quasar lensed by a gas-rich galaxy.
o	The lens galaxy is later identified as [WWL2003] QSO J0514-3326 abs 0.9313.
o	Table 1: <[GWB2000] 0512-3329 A> (Nos A-B). Table 2: <[GWB2000] Star N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWB2009]
[GWB2009]	(Gray+Wolf+Barden+, 2009)
Write:	<<[GWB2009] NNNNN>>
N:	63775
Object:	Unknown (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST ACS Photometry of the complex multicluster system A901/2. Use of archival XMM-Newton, GALEX, Spitzer, GMRT, and COMBO-17 data. See also COMBO.
in source:	NAME ACO 901-902 Supercluster
Ref:	=2009MNRAS.393.1275G
by	GRAY M.E. , WOLF C., BARDEN M., PENG C.Y., HAUSSLER B., BELL E.F., McINTOSH D.H., GUO Y., CALDWELL J.A.R., BACON D., BALOGH M., BARAZZA F.D., BOHM A., HEYMANS C., JAHNKE K., JOGEE S., VAN KAMPEN E., LANE K., MEISENHEIMER K., SANCHEZ S.F., TAYLOR A., WISOTZKI L., ZHENG X., GREEN D.A., BESWICK R.J., SAIKIA D.J., GILMOUR R., JOHNSON B.D., PAPOVICH C.
	Mon. Not. R. Astron. Soc., 393, 1275-1301 (2009)
	STAGES: the Space Telescope A901/2 Galaxy Evolution Survey.
o	<STAGES FF-NNNN> N=75805. <COMBO JHHMMSSs+DDMMSS> = <[GWB2009] NNNNN> N=63775.
=E=	Catalogue in electronic form as J/MNRAS/393/1275
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWC2000]
[GWC2000]	(Gorjian+Wright+Chary, 2000)
Write:	<<[GWC2000] ANNN>>
N:	28
Object:	* (SIMBAD class: Star)
Note:	N=28 bright stars in a dark spot near the NGP.
Ref:	=2000ApJ...536..550G
by	GORJIAN V. , WRIGHT E.L., CHARY R.R.
	Astrophys. J., 536, 550-560 (2000)
	Tentative detection of the cosmic infrared background at 2.2 and 3.5 microns using ground-based and space-based observations.
o	Table 1: <[GWC2000] ANNN> N=28 among 302.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWC92]
[GWC92]	(Garrett+Walsh+Carswell, 1992)
Write:	<<[GWC92] RNN>>
N:	22
Object:	G (SIMBAD class: Galaxy)
Note:	N=22 galaxies among (Nos R1-R33) (letter 'R' for Rank) in the field of the lens system QSO 0957+561. See also YGKOW, [RGH85], [BTK93], [ACL97], [BFT97], [BLF99], [PMN99], [SOS99], [TF99].
Ref:	=1992MNRAS.254p..27G
by	GARRETT M.A. , WALSH D., CARSWELL R.F.
	Mon. Not. R. Astron. Soc., 254, part no 16, 27-31 (1992)
	Redshift measurements of the brightest cluster galaxies of the gravitational lens 0957+561.
o	G1 = YGKOW G1
o	Table 1: <[GWC92] RNN> N=22 among (Nos R1-R33).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWC93]
[GWC93]	(Gray+Whiteoak+Cram+, 1993)= (E) = (SgrE)
Write:	<<[GWC93] NN>>
N:	70
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
in source:	NAME Sgr E
Ref:	=1993MNRAS.264..678G
by	GRAY A.D. , WHITEOAK J.B.Z., CRAM L.E., GOSS W.M.
	Mon. Not. R. Astron. Soc., 264, 678-682 (1993)
	Radio continuum observations of Sgr E.
o	Table 1: <[GWC93] NN> (Nos 1-70).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWC99]
[GWC99]	(Garnett+Walsh+Chu+, 1999)= (BG)
Write:	<<[GWC99] BG JHHMMSS+DDMMSS>>
N:	5
Object:	Bok Globule (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations. Rounded format.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1999AJ....117.1285G
by	GARNETT D.R. , WALSH J.R., CHU Y.-H., LASKER B.M.
	Astron. J., 117, 1285-1291 (1999)
	Bok globules in the Large Magellanic Cloud.
o	Table 2: <[GWC99] BG JHHMMSS-DDMMSS> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWH91]
[GWH91]	(Giovanelli+Williams+Haynes, 1991)
Write:	<<[GWH91] HI 1225+01 WW>>
N:	2
Object:	Clump (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	Arecibo HI observations of the HI 1225+01 cloud.
in source:	NAME HI 1225+01
Ref:	=1991AJ....101.1242G
by	GIOVANELLI R. , WILLIAMS J.P., HAYNES M.P.
	Astron. J., 101, 1242-1257 (1991)
	A complete Arecibo map of H I 1225+01.
o	Table 1: <[GWH91] HI 1225+01 WW> (Nos NE, SW).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWJ2008]
[GWJ2008]	(Guan+Wu+Ju, 2008)
Write:	<<[GWJ2008] HHMMm+DDMM-N>> <<[GWJ2008] S146>> <<[GWJ2008] S270-N>>
N:	53
Object:	CO Core (SIMBAD class: MolCld = Molecular Cloud)
Note:	Purple Moutain Observatory 13.7m telescope CO line observations of N=21 star-forming regions.
Ref:	=2008MNRAS.391..869G
by	GUAN X. , WU Y., JU B.
	Mon. Not. R. Astron. Soc., 391, 869-880 (2008)
	A mapping survey of massive CO cores.
o	Table 2: excluded regions are not in SIMBAD.
o	Table 1: <[GWJ2008] HHMMm+DDMM-N> N=50, <[GWJ2008] S146> N=1, <[GWJ2008] S270-N> (Nos 1-2).
=E=	Catalogue in electronic form as J/MNRAS/391/869
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWJ95]
[GWJ95]	(Gilmore+Wyse+Jones, 1995)
Write:	<<[GWJ95] HHMMSS.ss+DDMMSS.s>>
N:	133+87
Object:	* (SIMBAD class: Star)
Note:	Table 2: SGP fields stars, N=133. Table 4: F117 fields stars, N=87.
Ref:	=1995AJ....109.1095G
by	GILMORE G. , WYSE R.F.G., JONES J.B.
	Astron. J., 109, 1095-1111 (1995)
	A determination of the thick disk chemical abundance distribution: implications for galaxy evolution.
o	Tables 2, 4: <[GWJ95] HHMMSS.ss-DDMMSS.s> N=133+87
=E=	Catalogue in electronic form as J/AJ/109/1095
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWK2020]
[GWK2020]	(Gilbert+Wojno+Kirby+, 2020)
Write:	<<[GWK2020] And R NNNNNNN>>
N:	21
Object:	* (SIMBAD class: Star)
Note:	Keck II DEIMOS spectroscopic observations of N=21 M31 outer halo stars.
in source:	M 31 = NGC 224
Ref:	=2020AJ....160...41G
by	GILBERT K.M. , WOJNO J., KIRBY E.N., ESCALA I., BEATON R.L., GUHATHAKURTA P., MAJEWSKI S.R.
	Astron. J., 160, 41-41 (2020)
	Elemental abundances in M31: iron and α element abundances in M31's outer halo.
o	Table 1: <[GWK2020] And R NNNNNNN> N=21.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWM2004]
[GWM2004]	(Gorjian+Werner+Mould+, 2004)= ([GWM2004a])
Write:	<<[GWM2004] He 206 Bar>> <<[GWM2004] He 206 R>>
N:	1+3
Object:	Em. Region (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Spitzer Space Telescope, CTIO, and Gemini IR observations of the star-forming region He 206 (= LHA 120-N 206). The 3 brightest emitting regions are labeled I to III, and the overall star formation bar is a 11'x7' region.
in source:	Magellanic Clouds:LMC:LHA 120-N 206 = LHA 120-N 206
Ref:	=2004ApJS..154..275G
by	GORJIAN V. , WERNER M.W., MOULD J.R., GORDON K.D., MUZZEROLE J., MORRISON J., SURACE J.M., REBULL L.M., HURT R.L., SMITH R.C., POINTS S.D., AGUILERA C., DE BUIZER J.M., PACKHAM C.
	Astrophys. J., Suppl. Ser., 154, 275-280 (2004)
	Infrared imaging of the Large Magellanic Cloud star-forming region Henize 206.
o	Table 1, Figs 1, 2: <[GWM2004] He 206 Bar> N=1, <[GWM2004] He 206 R> (Nos I to III).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWM2004a]
[GWM2004a]	(Gorjian+Werner+Mould+, 2004)
*****	Avoid the usage of [GWM2004a], prefer [GWM2004]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWM2004b]
[GWM2004b]	(Gioia+Wolter+Mullis+, 2004)
Write:	<<[GWM2004b] NN>>
N:	20
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	CFHT and Keck-I spectroscopy of galaxies in RX J1821.6+6827.
in source:	RX J1821.0+6827
Ref:	=2004A&A...428..867G
by	GIOIA I.M. , WOLTER A., MULLIS C.R., HENRY J.P., BOEHRINGER H., BRIEL U.G.
	Astron. Astrophys., 428, 867-875 (2004)
	RXJ1821.6+6827: A cool cluster at z=0.81 from the ROSAT NEP survey.
o	Table 1: <[GWM2004b] NN> (Nos 1-20).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWM2005]
[GWM2005]	(Garrett+Wrobel+Morganti, 2005)
Write:	<<[GWM2005] NN>> <<[GWM2005] VLBI JHHMMSS.ssss+DDMMSS.sss>>
N:	61+10
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLBI observations of WSTR detected sources, using NRAO Long Baseline Array and 100m Green Bank Telescope in the NOAO Bootes field.
Ref:	=2005ApJ...619..105G
by	GARRETT M.A. , WROBEL J.M., MORGANTI R.
	Astrophys. J., 619, 105-115 (2005)
	Deep VLBI imaging of faint radio sources in the NOAO Bootes Field.
o	Tables 2-7: <[GWM2005] NN> (Nos 1-61), <[GWM2005] VLBI JHHMMSS.ssss+DDMMSS.sss> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWP2001]
[GWP2001]	(Gawiser+Wolfe+Prochaska+, 2001) (Not yet in Simbad)
Write:	<<[GWP2001] GN>>
N:	8
Object:	G (SIMBAD class: Galaxy)
Note:	N=8 confirmed galaxies with z>3.5 in the field of BR 0951-04.
Ref:	=2001ApJ...562..628G
by	GAWISER E. , WOLFE A.M., PROCHASKA J.X., LANZETTA K.M., YAHATA N., QUIRRENBACH A.
	Astrophys. J., 562, 628-634 (2001)
	First investigation of the clustering environment of damped Lyα absorbers at z≃4.
o	Table 3: <[GWP2001] GN> (Nos G1-G8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWP2017]
[GWP2017]	(Garofali+Williams+Plucinsky+, 2017)
Write:	<<[GWP2017] XMM-NNN>>
N:	218
Object:	Poss. SNR (SIMBAD class: SNRemnant_Candidate = SuperNova Remnant Candidate)
Note:	XMM-Newton observations of N=218 SNR candidates in M33.
in source:	NGC 598 = M 33
Ref:	=2017MNRAS.472..308G
by	GAROFALI K. , WILLIAMS B.F., PLUCINSKY P.P., GAETZ T.J., WOLD B., HABERL F., LONG K.S., BLAIR W.P., PANNUTI T.G., WINKLER P.F., GROSS J.
	Mon. Not. R. Astron. Soc., 472, 308-333 (2017)
	Supernova remnants in M33: X-ray properties as observed by XMM-Newton.
o	Table 2: <[GWP2017] XMM-NNN> (Nos 001-218).
=E=	Catalogue in electronic form as <J/MNRAS/472/308/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWS2009]
[GWS2009]	(Geha+Willman+Simon+, 2009)
Write:	<<[GWS2009] NNNNNNN>>
N:	51
Object:	* (SIMBAD class: Star)
Note:	Keck/DEIMOS spectroscopy of the Milky Way satellite Segue 1.
in source:	NAME Segue 1
Ref:	=2009ApJ...692.1464G
by	GEHA M. , WILLMAN B., SIMON J.D., STRIGARI L.E., KIRBY E.N., LAW D.R., STRADER J.
	Astrophys. J., 692, 1464-1475 (2009)
	The least-luminous galaxy: spectroscopy of the Milky Way satellite Segue 1.
o	Table 2, col(1): NNNNNNN are the last 7 digits of SDSS DR6 objID.
o	Table 2: <[GWS2009] NNNNNNN> N=51 among (Nos 1829185-3517219).
=E=	Catalogue in electronic form as <J/ApJ/692/1464/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWS2012]
[GWS2012]	(Guenther+Wolks+Spitzbart+, 2012)
Write:	<<[GWS2012] NNNNN>> <<[GWS2012] cluster core W>>
N:	40593+2
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Chandra, Spitzer and FLWO 1.2m telescope observations of the young star-forming region IRAS 20050+2720. Use of archival 2MASS and IPHAS data.
in source:	NAME IRAS 20050+2720 Cluster
Ref:	=2012AJ....144..101G
by	GUENTHER H.M. , WOLK S.J., SPITZBART B., GUTERMUTH R.A., FORBRICH J., WRIGHT N.J., ALLEN L., BOURKE T.L., MEGEATH S.T., PIPHER J.L.
	Astron. J., 144, 101 (2012)
	IRAS 20050+2720: anatomy of a young stellar cluster.
o	Table 3: <[GWS2012] NNNNN> (Nos 1-40593). Fig. 6, Paragr. 4.1: <[GWS2012] cluster core W> (Nos E, W).
=E=	Catalogue in electronic form as <J/AJ/144/101/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWS2014]
[GWS2014]	(Gomez+Wyrowski+Schuller+, 2014)
Write:	<<[GWS2014] GLLL.ll+BB.b>> <<[GWS2014] JHHMMSS.s+DDMMSS>> <<[GWS2014] GLLL>> (not recognised by Simbad, but found in literature)
N:	6+510+352
Object:	IRDC + Clump (SIMBAD class: FarIR = Far-IR source (λ >= 30 µm))
Note:	APEX LABOCA 870µm observations of N=6 infrared dark clouds (IRDCs), and N=510+352 clumps.
Ref:	=2014A&A...561A.148G
by	GOMEZ L. , WYROWSKI F., SCHULLER F., MENTEN K.M., BALLESTEROS-PAREDES J.
	Astron. Astrophys., 561A, 148-148 (2014)
	The mass distribution of clumps within infrared dark clouds. A large APEX Bolometer Camera study.
o	Paragraph 2.2 source 18592+0109 not identified. Paragraph 4.5 IRAS 17010-4124 not in SIMBAD.
o	Figs 1-2, Table 1: <[GWS2014] GLLL.ll+BB.b> N=6. Tables 3-4: <[GWS2014] JHHMMSS.s+DDMMSS> N=510+352.
=E=	Catalogue in electronic form as J/A+A/561/A148
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWS2018]
[GWS2018]	(Garling+Willman+Sand+, 2018)
Write:	<<[GWS2018] VNN>>
N:	3
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Stat:	is completely incorporated in Simbad
Note:	CTIO Blanco telescope DECam and Steward Observatory 2.3m Bok telescope observations of N=3 RR Lyrae stars in the field of the ultra-faint dwarf galaxy Hercules. Use of archival Beijing-Arizona Sky Survey. See also [MRM2012].
in source:	NAME Her Dwarf Galaxy
Ref:	=2018ApJ...852...44G
by	GARLING C. , WILLMAN B., SAND D.J., HARGIS J., CRNOJEVIC D., BECHTOL K., CARLIN J.L., STRADER J., ZOU H., ZHOU X., NIE J., ZHANG T., ZHOU Z., PENG X.
	Astrophys. J., 852, 44-44 (2018)
	Mapping the tidal destruction of the Hercules dwarf: a wide-field DECam imaging search for RR Lyrae stars.
o	In table 2, misprint in the coordinate of V1: read 16:31:02.17 instead of 16:21:02.17
o	Table 2: <[GWS2018] VNN> (Nos V11-V13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWS2022]
[GWS2022]	(Gull+Weisz+Senchyna+, 2022)
Write:	<<[GWS2022] KN>> <<[GWS2022] BNN>>
N:	8+14
Object:	OB* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Keck LRIS and MMT Binospec spectroscopy of N=8+14 OB stars in the Leo A galaxy. In the formats, K indicates Keck stars, B Binospec stars.
in source:	NAME Leo A
Ref:	=2022ApJ...941..206G
by	GULL M. , WEISZ D.R., SENCHYNA P., SANDFORD N.R., CHOI Y., McLEOD A.F., EL-BADRY K., GOTBERG Y., GILBERT K.M., BOYER M., DALCANTON J.J., GUHATHAKURTA P., GOLDMAN S., MARIGO P., McQUINN K.B.W., PASTORELLI G., STARK D.P., SKILLMAN E., TING Y.-S., WILLIAMS B.F.
	Astrophys. J., 941, 206 (2022)
	A Panchromatic Study of Massive Stars in the Extremely Metal-poor Local Group Dwarf Galaxy Leo A.
o	Fig. 3, Table 1: <[GWS2022] KN> (Nos K1-K8), <[GWS2022] BNN> (Nos B1-B14).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [GWS86]
[GWS86]	(Gledhill+Warren-Smith+Scarrott, 1986) (Not yet in Simbad)
Write:	<<[GWS86] Haro 6-5C>>
N:	1
Object:	* (SIMBAD class: Star)
Note:	N=1 star in the Haro 6-5 complex. See also [MBF84].
Ref:	=1986MNRAS.223..867G
by	GLEDHILL T.M. , WARREN-SMITH R.F., SCARROTT S.M.
	Mon. Not. R. Astron. Soc., 223, 867-875 (1986)
	Structure of the Haro 6-5 complex.
o	<[GWS86] Haro 6-5C> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWT2004]
[GWT2004]	(Grady+Woodgate+Torres+, 2004)
Write:	<<[GWT2004] HD 104237-N>>
N:	6
Object:	(Near IR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Stat:	is completely incorporated in Simbad
Note:	Multiwavelength observations of sources in the immediate vicinity of HD 104237 (HST/STIS, ESO NACO, ESO 3.6m La Silla).
Ref:	=2004ApJ...608..809G
by	GRADY C.A. , WOODGATE B., TORRES C.A.O., HENNING T., APAI D., RODMANN J., WANG H., STECKLUM B., LINZ H., WILLIGER G.M., BROWN A., WILKINSON E., HARPER G.M., HERCZEG G.J., DANKS A., VIEIRA G.L., MALUMUTH E., COLLINS N.R., HILL R.S.
	Astrophys. J., 608, 809-830 (2004)
	The environment of the optically brightest Herbig Ae star, HD 104237.
o	Table 2: <[GWT2004] HD 104237-N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWT2016]
[GWT2016]	(Ge+Wang+Tripp+, 2016)
Write:	<<[GWT2016] A1095 NN>> <<[GWT2016] A1926 NN>>
N:	47+78
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton EPIC observations N=47+78 sources in the ACO 1095 and ACO 1926 galaxy clusters. Use of archival SDSS, NVSS and FIRST data.
in source:	ACO 1926
in source:	ACO 1095
Ref:	=2016MNRAS.459..366G
by	GE C. , WANG Q.D., TRIPP T.M., LI Z., GU Q., JI L.
	Mon. Not. R. Astron. Soc., 459, 366-386 (2016)
	Baryon content and dynamic state of galaxy clusters: XMM-Newton observations of A1095 and A1926.
o	Table 3: <[GWT2016] A1095 NN> (Nos 1-47). Table 4: <[GWT2016] A1926 NN> (Nos 1-78).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWV98]
[GWV98]	(Gaume+Wilson+Vrba+, 1998)= (OMC-1S)
Write:	<<[GWV98] HHMMSS.sss+DDMMSS.ss>> <<[GWV98] A>>
N:	182+3
Object:	H2O Maser + (NIR) (SIMBAD class: Maser)
Note:	VLA (radio) and USNO IRCAM (NIR) observations. Tables 1, 2: H2O masers in Orion BN/KL and Orion. Table 3: (Nos A-C), N=3 compact near-IR sources, see Fig.6
in source:	NAME Orion Nebula
Ref:	=1998ApJ...493..940G
by	GAUME R.A. , WILSON T.L., VRBA F.J., JOHNSTON K.J., SCHMID-BURGK J.
	Astrophys. J., 493, 940-949 (1998)
	Water masers in Orion.
o	Tables 1-2: <[GWV98] HHMMSS.sss-DDMMSS.ss> N=146+36. Table 3: <[GWV98] A> (Nos A-C).
=E=	Catalogue in electronic form as <J/ApJ/493/940/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GWW98]
[GWW98]	(Gomez+Whitney+Wood, 1998)
Write:	<<[GWW98] HH 224 WWN>> <<[GWW98] ANa>>
N:	2+5
Object:	? (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Tables 1, 2: N=2 knots in HH 224, format 'HH 224 NW1' and 'HH 224 NW2'. N=5 candidates HH obj.: (Nos A1-A3, A4a-A4b).
in source:	NAME rho Oph Cloud
Ref:	=1998AJ....115.2018G
by	GOMEZ M. , WHITNEY B.A., WOOD K.
	Astron. J., 115, 2018-2027 (1998)
	A survey of optical jets and Herbig-Haro objects in the ρ Ophiuchi cloud core.
o	ROX 20-1 and 20-2 = ROXs 20A and B
o	Table 1: <HH NNN> (Nos 417-420). Tables 1, 2: <[GWW98] HH 224 WWN> (NosNW1, NW2), <[GWW98] ANa> (Nos A1-A3, A4a-A4b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Gwyn
Gwyn	(Gwyn) (Not yet in Simbad)
Write:	<<Gwyn HDFN NNNN>> <<Gwyn HDFN sN>> <<Gwyn HDFS NNN>> <<Gwyn HDFS sNN>>
N:	1015+6+886+11
Object:	G (SIMBAD class: Galaxy)
Note:	Gwyn catalogue of photometric redshifts in the HDFN and the HDFS: HDFN http://astrowww.phys.uvic.ca/~gwyn/pz/hdfn/spindex.htmlbr HDFS http://astrowww.phys.uvic.ca/~gwyn/pz/hdfs/spindex.htmlbr Some objects are found in 2001ApJ...561..106M.
in source:	NAME HDFN
in source:	NAME HDFS
Auth.:	GWYN S.D.J.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GX
GX	(Gal. X-ray source)
Write:	<<GX LLL.l+BB.b>> <<GX LLL+BB>> <<GX LLL.l+BB>> <<GX LLL+BB.b>> <<GX LLL.l>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Details on Acronym: [GXC2015]
[GXC2015]	(Gao+Xu+Chen, 2015)
Write:	<<[GXC2015] DDD.ddddd+DD.ddddd>>
N:	537
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Use of a clustering algorithm to identify N=537 3D cluster member stars in the open cluster NGC 6819.
in source:	NGC 6819
Ref:	=2015RAA....15.2193G
by	GAO X.-H. , XU S.-K., CHEN L.
	RAA, 15, 2193-2203 (2015)
	3D cluster members and near-infrared distance of open cluster NGC 6819.
o	Table 2 object KIC in SIMBAD.
o	Table 1: <[GXC2015] DDD.ddddd+DD.ddddd> N=537.
=E=	Catalogue in electronic form as J/other/RAA/15.2193
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GXL2018]
[GXL2018]	(Guo+Xin+Liao+, 2018)
Write:	<<[GXL2018] Newpts A>> <<[GXL2018] Source A>>
N:	7
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	N=7 gamma-ray sources in the supernova remnant HESS J1731-347. Use of Fermi Large Area Telescope (LAT) data.
Ref:	=2018ApJ...853....2G
by	GUO X.-L. , XIN Y.-L., LIAO N.-H., YUAN Q., GAO W.-H., FAN Y.-Z.
	Astrophys. J., 853, 2-2 (2018)
	Detection of GeV γ-ray emission in the direction of HESS J1731-347 with Fermi-LAT.
o	Table 1: <[GXL2018] Source T> N=1, <[GXL2018] Newpts A> (Nos A-F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Gy
Gy	(Gyulbudaghian)
*****	Avoid the usage of Gy, prefer [G82a]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: Gy
Gy	(Gyulbudaghian)
*****	Avoid the usage of Gy, prefer [G82b]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Gy
Gy	(Gyulbudaghian)
*****	Avoid the usage of Gy, prefer [G84b]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: Gy
Gy	(Gyulbudaghian)
*****	Avoid the usage of Gy, prefer [G84c]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: GY
GY	(Greene+Young)
*****	Avoid the usage of GY, prefer [GY92]
Origin	of the Acronym: L (1996AJ....112.2184G)
Details on Acronym: Gy
Gy	(Gyulbudaghian)
*****	Avoid the usage of Gy, prefer [TRC83]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GY84]
[GY84]	(Green+Yee, 1984)
Write:	<<[GY84] PHL 658 NN>> <<[GY84] PKS HHMM+DD NNA>> <<[GY84] PKS HHMM+DDd NNA>> <<[GY84] 4C DD.NN NNA>> <<[GY84] 3C NNN.N NNA>> <<[GY84] PG HHMM+DD NNA>>
N:	2837
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=2837 nearby objects of 108 QSOs. See also [YGS86].
Ref:	=1984ApJS...54..495G
by	GREEN R.F. , YEE H.K.C.
	Astrophys. J., Suppl. Ser., 54, 495-512 (1984)
	An imaging survey of fields around quasars. I. A catalog.
o	Table 2: <[GY84] PHL 658 NN>, <[GY84] PKS HHMM+DD NNA>, <[GY84] PKS HHMM+DDd NNA>, <[GY84] 4C DD.NN NNA>, <[GY84] 3C NNN NNA>, <[GY84] 3C NNN.N NNA>, N=2774.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GY92]
[GY92]	(Greene+Young, 1992)= (GY) = (IRS)
Write:	<<[GY92] NNN>>
N:	481
Object:	(IR) (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Rem:	no plates
in source:	NAME rho Oph Cloud
Ref:	=1992ApJ...395..516G
by	GREENE T.P. , YOUNG E.T.
	Astrophys. J., 395, 516-528 (1992)
	Near-infrared observations of young stellar objects in the ρ Ophiuchi dark cloud.
o	<[GY92] NNN> (Nos 1-481).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GYE2002]
[GYE2002]	(Gladders+Yee+Ellingson, 2002)
Write:	<<[GYE2002] J0224-0002 AN>> <<[GYE2002] J0224-0002 RN>>
N:	4+7+2
Object:	Arc (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Stat:	is completely incorporated in Simbad
Note:	N=4 tangential arc-like structures (Nos A-D), A and B with components 'AN', and 2 radial arc candidates (Nos R1-R2) which are potentially lensed background sources, lensed by RCS J0224-0002. See also [SBS2007].
Ref:	=2002AJ....123....1G
by	GLADDERS M.D. , YEE H.K.C., ELLINGSON E.
	Astron. J., 123, 1-9 (2002)
	Discovery of a z =0.77 galaxy cluster with multiple, bright, strong-lensing arcs.
o	Text: <RCS JHHMM+DDMM> N=1. Table 1, Fig.2: <[GYE2002] J0224-0002 A> (Nos A-D). Fig.3: <[GYE2002] J0224-0002 AN> (Nos R1-R2).
Ref:	=2007A&A...471..743R
by	RZEPECKI J. , LOMBARDI M., ROSATI P., BIGNAMINI A., TOZZI P.
	Astron. Astrophys., 471, 743-752 (2007)
	Strong lensing analysis of the cluster RCS 0224-0002 at z = 0.77.
o	Fig.1: <[GYE2002] J0224-0002 AN> (Nos A1-A3, B1-B4) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GYO2019]
[GYO2019]	(Gim+Yun+Owen+, 2019)
Write:	<<[GYO2019] GW-NNa>>
N:	143
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Jansky Very Large Array 5GHz observations of N=143 sources in the GOODS South and North fields.
in source:	NAME GOODS South Field
in source:	NAME GOODS North Field
Ref:	=2019ApJ...875...80G
by	GIM H.B. , YUN M.S., OWEN F.N., MOMJIAN E., MILLER N.A., GIAVALISCO M., WILSON G., LOWENTHAL J.D., ARETXAGA I., HUGHES D.H., MORRISON G.E., KAWABE R.
	Astrophys. J., 875, 80-80 (2019)
	Nature of faint radio sources in GOODS-North and GOODS-South fields. I. Spectral index and Radio-FIR correlation.
o	Table 2: <[GYO2019] GW-NNa> N=143 among (Nos GS-01 to GS-83, GN-01 to GN-52).
=E=	Catalogue in electronic form as <J/ApJ/875/80/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GZ
GZ	(Gunn Z band)
Write:	<<GZ A>>
N:	2
Object:	(Rad) (SIMBAD class: Unknown = Object of Unknown Nature)
in source:	NAME Gal Center
Ref:	=1992A&A...257..515R
by	ROSA M.R. , ZINNECKER H., MONETI A., MELNICK J.
	Astron. Astrophys., 257, 515-522 (1992)
	The Galactic Center in the Far-Red.
o	Table 3: <GCIRS NNA> No. 12C is new, <GZ A> (Nos A-B)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [GZB2006]
[GZB2006]	(Gonzalez-Garcia+Zapatero Osorio+Bejar+, 2006)= (Prae)
Write:	<<[GZB2006] Prae JHHMMSS.s+DDMMSS>>
N:	20
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Sloan i' and z' photometry at the Calar Alto 3.5m and the Palomar Observatories' 5m Hale telescopes of the Praesepe star cluster.
in source:	NAME Praesepe
Ref:	=2006A&A...460..799G
by	GONZALEZ-GARCIA B.M. , ZAPATERO OSORIO M.R., BEJAR V.J.S., BIHAIN G., BARRADO Y NAVASCUES D., CABALLERO J.A., MORALES-CALDERON M.
	Astron. Astrophys., 460, 799-810 (2006)
	A search for substellar members in the Praesepe and σ Orionis clusters.
o	Table 5: <[GZB2006] Prae JHHMMSS.s+DDMMSS> N=20. Table 6: <[BMZ2001] S Ori JHHMMSS.s+DDMMSS> N=18 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GZC2016]
[GZC2016]	(Grasshorn Gebhardt+Zeimann+Ciardullo+, 2016)
Write:	<<[GZC2016] NNN>>
N:	256
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=256 emission-line galaxies from the HST grism surveys of the COSMOS, GOODS-North and GOODS-South fields.
in source:	NAME COSMOS Field
in source:	NAME GOODS North Field
in source:	NAME GOODS South Field
Ref:	=2016ApJ...817...10G
by	GRASSHORN GEBHARDT H.S. , ZEIMANN G.R., CIARDULLO R., GRONWALL C., HAGEN A., BRIDGE J.S., SCHNEIDER D.P., TRUMP J.R.
	Astrophys. J., 817, 10 (2016)
	Young, star-forming galaxies and their local counterparts: the evolving relationship of mass-SFR-metallicity since z ~ 2.1.
o	Tables 1-2: <[GZC2016] NNN> (Nos 1-256).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GZD97]
[GZD97]	(Gruppioni+Zamorani+De Ruiter+, 1997)
Write:	<<[GZD97] 1.4 NNA>> <<[GZD97] 2.4 NNA>>
N:	74+58
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 1: format '1-NNA', 1.4 GHz sample, N=74 Table 2: format '2-NNA', 2.4 GHz sample, N=58 Table 4: 43 objects are the same in the 2 tables (cross-id), N of objects = 89.
Ref:	=1997MNRAS.286..470G
by	GRUPPIONI C. , ZAMORANI G., DE RUITER H.R., PARMA P., MIGNOLI M., LARI C.
	Mon. Not. R. Astron. Soc., 286, 470-482 (1997)
	Radio observations of the Marano Field and the faint radio galaxy population.
o	Table 1: <[GZD97] 1.4 NNA> N=74, (Nos 1-63). Table 2: <[GZD97] 2.4 NNA> N=58, (Nos 1-48).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: GZG
GZG	(Gil de Paz+Zamorano+Gallego)
*****	Avoid the usage of GZG, prefer [GZG99]
Origin	of the Acronym: A (2000A&AS..145..377G)
Details on Acronym: [GZG2000]
[GZG2000]	(Gil de Paz+Zamorano+Gallego+, 2000)
Write:	<<[GZG2000] NN>>
N:	85
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Knots in Mrk 86. A first knot numbering is used in [GZG99].
in source:	Mrk 86
Ref:	=2000A&AS..145..377G
by	GIL DE PAZ A. , ZAMORANO J., GALLEGO J., DOMINGUEZ F. DE B.
	Astron. Astrophys., Suppl. Ser., 145, 377-397 (2000)
	Mapping the star formation history of Mrk 86. I. Data and models.
o	Table 3: <[GZG2000] NN> (Nos 1-85).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GZG99]
[GZG99]	(Gil de Paz+Zamorano+Gallego, 1999)= (GZG)
Write:	<<[GZG99] NN>>
N:	55
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
Note:	First numbering for knots in Mrk 86. This numbering is used in col(2), 2000A&AS..145..377G. See [GZG2000].
in source:	Mrk 86
Ref:	=1999MNRAS.306..975G
by	GIL DE PAZ A. , ZAMORANO J., GALLEGO J.
	Mon. Not. R. Astron. Soc., 306, 975-987 (1999)
	Global velocity field and bubbles in the blue compact dwarf galaxy Mrk 86.
o	Table 3: <[M98b] NGC 2537-A> (Nos B, C) added. Text, Figs: <[GZG99] NN> N=4 among (Nos 1-55).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GZK2003]
[GZK2003]	(Gusev+Zasov+Kaisin, 2003) (Not yet in Simbad)
Write:	<<[GZK2003] NN>>
N:	11
Object:	Region (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Photometry of NGC 4136. N=11 regions of star formation are found.
in source:	NGC 4136
Ref:	=2003AstL...29..363G
by	GUSEV A.S. , ZASOV A.V., KAISIN S.S.
	Astron. Lett., 29, 363-371 (2003)
	Photometry of the low-luminosity spiral galaxy NGC 4136.
o	Table 3: <[GZK2003] NN> (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GZK2010]
[GZK2010]	(Galvan-Madrid+Zhang+Keto+, 2010)
Write:	<<[GZK2010] MMN-Main>> <<[GZK2010] MMN-WW>> <<[GZK2010] MM1-Ridge>>
N:	2+5+1
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	2010ApJ...725...17G: SMA 1.3mm and 0.9mm continuum observations of N=5 sources in the W33A massive star formation region. 2017MNRAS.467L.120M: ALMA band 6 (230GHz) and 7 (345GHz) observations of N=3 sources in [VVE2000] W33A MM 1.
in source:	W 33:W 33A = W 33A
Ref:	=2010ApJ...725...17G
by	GALVAN-MADRID R. , ZHANG Q., KETO E., HO P.T.P., ZAPATA L.A., RODRIGUEZ L.F., PINEDA J.E., VAZQUEZ-SEMADENI E.
	Astrophys. J., 725, 17-28 (2010)
	From the convergence of filaments to disk-outflow accretion: massive star formation in W33A.
o	Table 2: <[GZK2010] MMN-Main> (Nos MM1-Main and MM2-Main), <[GZK2010] MMN-WW> (Nos MM1-NW, MM1-SE, MM2-NE).
Ref:	=2017MNRAS.467L.120M
by	MAUD L.T. , HOARE M.G., GALVAN-MADRID R., ZHANG Q., DE WIT W.J., KETO E., JOHNSTON K.G., PINEDA J.E.
	Mon. Not. R. Astron. Soc., 467L, 120-124 (2017)
	The ALMA view of W33A: a spiral filament feeding the candidate disc in MM1-Main.
o	Fig. 1, Table 1: <[GZK2010] MM1-W> (Nos E, S) added, <[GZK2010] MM1-Ridge> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GZR2015]
[GZR2015]	(Glushkova+Zabolotskikh+Rastorguev+, 2015)
Write:	<<[GZR2015] OSC DDD.ddddd+DD.ddddd>>
N:	8
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	N=8 open star clusters (OSCs) identified in a search for young star clusters and associations near known Cepheids. Use of 2MASS data.
Ref:	=2015BaltA..24..360G
by	GLUSHKOVA E.V. , ZABOLOTSKIKH M.V., RASTORGUEV A.S., GRUDSKAYA A.V.
	BaltA, 24, 360-366 (2015)
	A search for new open clusters hosting cepheids.
o	Table 1, Paragr. 3: <[GZR2015] OSC DDD.ddddd+DD.ddddd> N=4+4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GZS2022]
[GZS2022]	(Gran+Zoccali+Saviane+, 2022) (Not yet in Simbad)
Write:	<<[GZS2022] C1>>
N:	1
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	VLT MUSE spectroscopy of N=1 candidate globular cluster towards the Galactic bulge. Use of Gaia (DR2 and EDR3) data, and VVV data.
Ref:	=2022MNRAS.509.4962G
by	GRAN F. , ZOCCALI M., SAVIANE I., VALENTI E., ROJAS-ARRIAGADA A., CONTRERAS RAMOS R., HARTKE J., CARBALLO-BELLO J.A., NAVARRETE C., REJKUBA M., OLIVARES CARVAJAL J.
	Mon. Not. R. Astron. Soc., 509, 4962-4981 (2022)
	Hidden in the haystack: low-luminosity globular clusters towards the Milky Way bulge.
o	Table 1: <Gran N> (Nos 2-5), <[GZS2022] C1> N=1.
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [GZW2002]
[GZW2002]	(Giacconi+Zirm+Wang+, 2002)= (CDFS)
Write:	<<[GZW2002] Main NNN>> <<[GZW2002] SExtractor NN>> <<[GZW2002] WAVDETECT NN>> <<[GZW2002] XID NNN>>
N:	346+3
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra Catalog of the CDFS. Table 2: Main catalog, format 'Main NNN', (Nos 1-304). Table 3: Objects observed only with SExtractor, format 'SExtractor NN', (Nos 1-28). Table 4: Objects observed only with WAVDETECT, format 'WAVDETECT NN', (Nos 1-14). Tables 2, 3, 4, col(2): Another format 'XID' is introduced by the authors N=304+28+14 among (Nos 1-653). See also CXOCDFS, [SBH2004]. In 2004ApJS..155..271S, [GZW2002] XID 901, 902, 903 are added.
in source:	NAME CDFS
Ref:	=2002ApJS..139..369G
by	GIACCONI R. , ZIRM A., WANG J., ROSATI P., NONINO M., TOZZI P., GILLI R., MAINIERI V., HASINGER G., KEWLEY L., BERGERON J., BORGANI S., GILMOZZI R., GROGIN N., KOEKEMOER A., SCHREIER E., ZHENG W., NORMAN C.
	Astrophys. J., Suppl. Ser., 139, 369-410 (2002)
	Chandra Deep Field South: the 1 Ms catalog.
o	CXOCDFS J033260.0-274748 translated into CXOCDFS J033300.0-274748
o	Table 2: <[GZW2002] Main NNN> (Nos 1-304) = <[GZW2002] XID NNN> N=304 = <CXOCDFS JHHMMSS.s+DDMMSS> N=304. Table 3: <[GZW2002] SExtractor NN> (Nos 1-28) = <[GZW2002] XID NNN> N=28 = <CXOCDFS JHHMMSS.s+DDMMSS> N=28. Table 4: <[GZW2002] WAVDETECT NN> (Nos 1-14) = <[GZW2002] XID NNN> N=14 = <CXOCDFS JHHMMSS.s+DDMMSS> N=14.
Ref:	=2004ApJS..155..271S
by	SZOKOLY G.P. , BERGERON J., HASINGER G., LEHMANN I., KEWLEY L., MAINIERI V., NONINO M., ROSATI P., GIACCONI R., GILLI R., GILMOZZI R., NORMAN C., ROMANIELLO M., SCHREIER E., TOZZI P., WANG J.X., ZHENG W., ZIRM A.
	Astrophys. J., Suppl. Ser., 155, 271-349 (2004)
	The Chandra Deep Field-South: Optical spectroscopy. I..
o	Tables 4, 8: <[SBH2004] JHHMMSS.ss+DDMMSS.s> N=288+139. Tables 4, 8: <[SBH2004] XID NNNa> N=103+50. Table 9: <[SBH2004] NNNNN> N=124 among (Nos 12-60041). Table 5: <[GZW2002] XID NNN> (Nos 901-903) added.
=E=	Catalogue in electronic form as J/ApJS/139/369
=E=	Catalogue in electronic form as J/ApJS/155/271
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GZW2003]
[GZW2003]	(Georgantopoulos+Zezas+Ward, 2003)
Write:	<<[GZW2003] JHHMMSS.s+DDMMSS>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of IRAS 00317-2142. N=2 point-source eastward of IRAS source.
Ref:	=2003ApJ...584..129G
by	GEORGANTOPOULOS I. , ZEZAS A., WARD M.J.
	Astrophys. J., 584, 129-134 (2003)
	X-Ray-Luminous galaxies. I. Chandra observations of IRAS 00317-2142.
o	Text: <[GZW2003] JHHMMSS.s+DDMMSS> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [GZZ2000]
[GZZ2000]	(Gonzalez+Zabludoff+Zaritsky+, 2000) (Not yet in Simbad)
Write:	<<[GZZ2000] A>>
N:	3
Object:	Region (SIMBAD class: Region = Region defined in the Sky)
Note:	N=3 regions of excess brightness in ACO 1651.
in source:	ACO 1651
Ref:	=2000ApJ...536..561G
by	GONZALEZ A.H. , ZABLUDOFF A.I., ZARITSKY D., DALCANTON J.J.
	Astrophys. J., 536, 561-570 (2000)
	Measuring the diffuse optical light in Abell 1651.
o	(Erratum) erratum vol. 611, p. 1208 (2004)
o	Fig.6: <[GZZ2000] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: H
H	(Higgs) (Not yet in Simbad)
*****	Avoid the usage of H, prefer Hig
Details on Acronym: H
H	(Hubble)
*****	Avoid the usage of H, prefer BASW
Origin	of the Acronym: L = Found in the literature
Details on Acronym: H
H	(Harten)
*****	Avoid the usage of H, prefer [BHJ77]
Origin	of the Acronym: L (1980A&A....90..246I)
Details on Acronym: H
H	(HDF)
*****	Avoid the usage of H, prefer [CSS2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: H
H	(HI Hole)
*****	Avoid the usage of H, prefer [DD90]
Origin	of the Acronym: L (2001PASJ...53..663O)
Details on Acronym: H
H	(Hyland+)
*****	Avoid the usage of H, prefer Dor
Origin	of the Acronym: L (1998A&A...331..857J)
Details on Acronym: H
H	(HEAO satellite)= (HEAO)
Write:	<<H HHMM+DD>> <<H HHMM+DDd>>
N:	60+114
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	1979ApJS...40..657M: N=60, 47 are new sources, All sky, Energy 3-17 keV. 1983ApJS...51....1N: N=114, 54 were previously undiscovered and 32 remain unidentified. The catalogue contains a listing of all counterpart identif. and a cross-reference to all HEAO 1 A-2 low energy detector team publications on the catalogue sources complete through the end of 1981.
Ref:	=1979ApJS...40..657M
by	MARSHALL F.E. , BOLDT E.A., HOLT S.S., MUSHOTZKY R.F., PRAVDO S.H., ROTHSCHILD R.E., SERLEMITSOS P.J.
	Astrophys. J., Suppl. Ser., 40, 657-666 (1979)
	New hard X-ray sources observed with HEAO A-2.
o	Table 2: <H HHMM+DDd> N=47
Ref:	=1983ApJS...51....1N
by	NUGENT J.J. , JENSEN K.A., NOUSEK J.A., GARMIRE G.P., MASON K.O., WALTER F.M., BOWYER C.S., STERN R.A., RIEGLER G.R.
	Astrophys. J., Suppl. Ser., 51, 1-28 (1983)
	HEAO A-2 soft X-ray source catalog.
o	Table 1: <H HHMM+DD> N=124
Details on Acronym: H
H	(HEAO satellite)= (H4) = (HEAO) = (HEAO 4-)
Write:	<<H HHMM+DDd>>
N:	72
Object:	(Hard X) (SIMBAD class: X = X-ray Source)
Note:	All sky. 4 channels in the 13-180keV range. Observations from 1977 August to 1979 January. Data obtained with the UCSD/MIT Hard X-ray and Low-Energy X-ray Instrument on the HEAO 1 satellite. The survey is complete down to an intensity level 1/75 of the Crab Nebulae in the 13-80 keV energy band. 44 sources detected in the 40-80 keV energy band. 7 sources are extragalactic.
Ref:	=1984ApJS...54..581L
by	LEVINE A.M. , LANG F.L., LEWIN W.H.G., PRIMINI F.A., DOBSON C.A., DOTY J.P., HOFFMAN J.A., HOWE S.K., SCHEEPMAKER A., WHEATON W.A., MATTESON J.L., BAITY W.A., GRUBER D.E., KNIGHT F.K., NOLAN P.L., PELLING R.M., ROTHSCHILD R.E., PETERSON L.E.
	Astrophys. J., Suppl. Ser., 54, 581-617 (1984)
	The HEAO1 A-4 catalog of high-energy X-ray sources.
o	Table 5: <H HHMM+DDd> N=72
Details on Acronym: H
H	(Hubble)
*****	Avoid the usage of H, prefer [H29]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: H
H	(Hubble)
*****	Avoid the usage of H, prefer [H32]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: H
H	(Hoffleit)
*****	Avoid the usage of H, prefer [H53]
Origin	of the Acronym: L (1974Ap&SS..27....3M)
Details on Acronym: H
H	(Hodge)
*****	Avoid the usage of H, prefer [H60b]
Details on Acronym: H
H	(Hodge)
*****	Avoid the usage of H, prefer [H65]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: H
H	(cloud complex labelled H)
*****	Avoid the usage of H, prefer [H68]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: H
H	(Hodge)
*****	Avoid the usage of H, prefer [H74b]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: H
H	(Hodge)
*****	Avoid the usage of H, prefer [H76]
Origin	of the Acronym: L (1999ApJ...510..104B)
Details on Acronym: H
H	(Hodge)
*****	Avoid the usage of H, prefer [H77]
Origin	of the Acronym: L (1980A&AS...40...67D)
Details on Acronym: H
H	(Hawkins)
*****	Avoid the usage of H, prefer [H83]
Origin	of the Acronym: L (Veron)
Details on Acronym: H
H	(Hubble Deep Field)
*****	Avoid the usage of H, prefer [HCB98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: H
H	(Hickson)
*****	Avoid the usage of H, prefer HCG
Origin	of the Acronym: L (1993ApJS...85....1N)
Details on Acronym: H
H	(Holtzman+)
*****	Avoid the usage of H, prefer [HFS92]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: H
H	(Hazard+)
*****	Avoid the usage of H, prefer [HMT84]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: H
H	(Hoglund)
*****	Avoid the usage of H, prefer NRAO
Details on Acronym: H
H	(Haddock)
*****	Avoid the usage of H, prefer NRL
Details on Acronym: H
H	(Haro)= H 1- = (Haro 2-). H 2- = (Haro 3-). H 3- = (Haro 6-)
Write:	<<PN H 1-NN>> <<PN H 2-NN>> <<PN H 3-NN>> <<PN H 4-N>>
N:	67+48+2+1
Object:	PN + Poss. PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	List 1: format '1-NN', table 1 in ref. 1952BOTT....1a...1H, H 1-25 and H 1-49 are rejected as PN in 1992, Acker+ catalog. List 2: format '2-NN', table 2 in ref. 1952BOTT....1a...1H, H 2-9 is a Nova. List 3: format '3-NN', two objects in ref. 1953BOTT....1h...3H are PN List4: format '4-N', in ref. 1951PASP...63..144H
Ref:	=1952BOTT....1a...1H
by	HARO G.
	Bol. Obs. Tonantz. Tacub., 1, part no 1, 1-None (1952)
	Nuevas nebulosas planetarias y objetos con emision en la region del centro galactico.
o	Table I: <PN H 1-NN> (Nos 1-1 to 1-67). Table II: <PN H 2-NN> (Nos 2-1 to 2-48).
Ref:	=1951PASP...63..144H
by	HARO G.
	Publ. Astron. Soc. Pac., 63, 144-145 (1951)
	Emission object in Coma.
o	PN H 4-1 = PK 049+88 1
o	<PN H 4-N> (No. 4-1).
Ref:	=1953BOTT....1h...3H
by	HARO G. , IRIARTE B., CHAVIRA E.
	Bol. Obs. Tonantz. Tacub., 1, part no 8, 3-18 (1953)
	Nuevas estrellas con emission en las regiones obscuras del Toro-Auriga-Orion investigadas por Joy.
o	Haro 6-29 = PN H 3-29, Haro 6-75 = PN H 3-75.
o	<Haro 6-NN> (Nos 6-1 to 6-75). <PN H 3-NN> N=2 (Nos 3-29, 3-75).
Details on Acronym: H
H	(Hoffleit)
*****	Avoid the usage of H, prefer Hf
Details on Acronym: H
H	(HI Hole)
*****	Avoid the usage of H, prefer [PWB92]
Origin	of the Acronym: L (1999AJ....118..323R)
Details on Acronym: H
H	(HRI obs.)
*****	Avoid the usage of H, prefer [SBF2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: H
H	(Harris)
====>	Equivalent to: [SRB2011]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: H
H	(Hubble)
*****	Avoid the usage of H, prefer [V62]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: H
H	(HST)
*****	Avoid the usage of H, prefer [VFK98]
Origin	of the Acronym: L (2007ApJ...661..750T)
Details on Acronym: H
H	(Hubble)
*****	Avoid the usage of H, prefer VHK
Origin	of the Acronym: L = Found in the literature
Details on Acronym: H-A
H-A	(Hodge Assoc.)
*****	Avoid the usage of H-A, prefer SMC Ass
Origin	of the Acronym: L = Found in the literature
Details on Acronym: H-ATLAS
H-ATLAS	(Herschel ATLAS)= (HATLAS)
Write:	<<H-ATLAS JHHMMSS.s+DDMMSS>> <<H-ATLAS HHMMSS.s+DDMMSS>> (not recognised by Simbad, but found in literature)
N:	about 200000
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	The Herschel ATLAS survey (http://www.h-atlas.org) is based on data from Herschel telescope (herschel.esac.esa.int). The aim is to map more than 500 square degrees in the pass bands centred on 100, 160, 250, 350 and 500 microns. The catalogue is the band-merged list of sources detected at more than 5-sigma level in any of the bands. The Herschel ATLAS survey is described in 2010PASP..122..499E.
Ref:	=2010Sci...330..800N
by	NEGRELLO M. , HOPWOOD R., DE ZOTTI G., COORAY A., VERMA A., BOCK J., FRAYER D.T., GURWELL M.A., OMONT A., NERI R., DANNERBAUER H., LEEUW L.L., BARTON E., COOKE J., KIM S., DA CUNHA E., RODIGHIERO G., COX P., BONFIELD D.G., JARVIS M.J., SERJEANT S., IVISON R.J., DYE S., ARETXAGA I., HUGHES D.H., IBAR E., BERTOLDI F., VALTCHANOV I., EALES S., DUNNE L., DRIVER S.P., AULD R., BUTTIGLIONE S., CAVA A., GRADY C.A., CLEMENTS D.L., DARIUSH A., FRITZ J., HILL D., HORNBECK J.B., KELVIN L., LAGACHE G., LOPEZ-CANIEGO M., GONZALEZ-NUEVO J., MADDOX S., PASCALE E., POHLEN M., RIGBY E.E., ROBOTHAM A., SIMPSON C., SMITH D.J.B., TEMI P., THOMPSON M.A., WOODGATE B.E., YORK D.G., AGUIRRE J.E., BEELEN A., BLAIN A., BAKER A.J., BIRKINSHAW M., BLUNDELL R., BRADFORD C.M., BURGARELLA D., DANESE L., DUNLOP J.S., FLEUREN S., GLENN J., HARRIS A.I., KAMENETZKY J., LUPU R.E., MADDALENA R.J., MADORE B.F., MALONEY P.R., MATSUHARA H., MICHALOWSKI M.J., MURPHY E.J., NAYLOR B.J., NGUYEN H., POPESCU C., RAWLINGS S., RIGOPOULOU D., SCOTT D., SCOTT K.S., SEIBERT M., SMAIL I., TUFFS R.J., VIEIRA J.D., VAN DER WERF P.P., ZMUIDZINAS J.
	Sci, 330, 800-804 (2010)
	The detection of a population of submillimeter-bright, strongly lensed galaxies.
o	Tables 1-2, Figs. 2-3: <SDP NNN> (Nos 9, 11, 17, 81, 130). Table S1: <H-ATLAS JHHMMSS.s+DDMMSS> N=5. Table 1: <[NHD2010] SDP NNN lens> N=5.
Ref:	=2016MNRAS.462.3146V
by	VALIANTE E. , SMITH M.W.L., EALES S., MADDOX S.J., IBAR E., HOPWOOD R., DUNNE L., CIGAN P.J., DYE S., PASCALE E., RIGBY E.E., BOURNE N., FURLANETTO C., IVISON R.J.
	Mon. Not. R. Astron. Soc., 462, 3146-3179 (2016)
	The Herschel-ATLAS data release 1 - I. Maps, catalogues and number counts.
o	<H-ATLAS JHHMMSS.s+DDMMSS> N=120230 = <[VSE2016] GHH.DR1.NNNNNN> N=120230 among (Nos G09.DR1.1-G09.DR1.169987, G12.DR1.1-G12.DR1.168280, G15.DR1.1-G15.DR1.175966).
Ref:	=2018ApJS..236...30M
by	MADDOX S.J. , VALIANTE E., CIGAN P., DUNNE L., EALES S., SMITH M.W.L., DYE S., FURLANETTO C., IBAR E., DE ZOTTI G., MILLARD J.S., BOURNE N., GOMEZ H.L., IVISON R.J., SCOTT D., VALTCHANOV I.
	Astrophys. J., Suppl. Ser., 236, 30-30 (2018)
	The Herschel-ATLAS data release 2. Paper II. Catalogs of far-infrared and submillimeter sources in the fields at the South and North Galactic Poles.
o	<H-ATLAS JHHMMSS.s+DDMMSS> N=118980 = <[MVC2018] NGP.DR2.NNNNNN> N=118980 among (Nos NGP.DR2.1-NGP.DR2.504529). <H-ATLAS JHHMMSS.s+DDMMSS> N=193527 = <[MVC2018] SGP.DR2.NNNNNN> N=193527 among (Nos SGP.DR2.1-SGP.DR2.825394).
Ref:	=2016ApJ...832...78I
by	IVISON R.J. , LEWIS A.J.R., WEISS A., ARUMUGAM V., SIMPSON J.M., HOLLAND W.S., MADDOX S., DUNNE L., VALIANTE E., VAN DER WERF P., OMONT A., DANNERBAUER H., SMAIL I., BERTOLDI F., BREMER M., BUSSMANN R.S., CAI Z.-Y., CLEMENTS D.L., COORAY A., DE ZOTTI G., EALES S.A., FULLER C., GONZALEZ-NUEVO J., IBAR E., NEGRELLO M., OTEO I., PEREZ-FOURNON I., RIECHERS D., STEVENS J.A., SWINBANK A.M., WARDLOW J.
	Astrophys. J., 832, 78-78 (2016)
	The space density of luminous dusty star-forming galaxies at z > 4: SCUBA-2 and LABOCA imaging of ultrared galaxies from Herschel-ATLAS.
o	Table 1, col(1): <H-ATLAS JHHMMSS.s+DDMMSS> N=109. Table 1, col(2): <[ILW2016] GHH-NNNNNN> N=47 among (Nos G09-47693 to G09-101355, G12-34009 to G12-87695, G15-21998 to G15-105504), <[ILW2016] SGP-NNNNNN> N=33 among (Nos 28124-499828), <[ILW2016] NGP-NNNNNN> N=32 among (Nos 63663-316031).
=E=	Catalogue in electronic form as <J/MNRAS/462/3146/>
=E=	Catalogue in electronic form as <J/ApJS/236/30/>
=E=	Catalogue in electronic form as <J/ApJ/832/78/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: H-C
H-C	(Haro+Chavira)
*****	Avoid the usage of H-C, prefer HaroChavira
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: H-K
H-K	(Heidelberg Konigstuhl obs.) (Not yet in Simbad)
*****	Avoid the usage of H-K, prefer [KS65]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: H-M
H-M	(Heydari-Malayeri+)
*****	Avoid the usage of H-M, prefer [HGM93]
Origin	of the Acronym: L (1999AJ....118.1684W)
Details on Acronym: H-M
H-M	(Heydari-Malayeri+)
*****	Avoid the usage of H-M, prefer [HT83]
Origin	of the Acronym: L (1999AJ....118.1684W)
Details on Acronym: H-S
H-S	(Hubble+Sandage)
*****	Avoid the usage of H-S, prefer [HS53]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: H-Z
H-Z	(Humason+Zwicky)
*****	Avoid the usage of H-Z, prefer HZ
Details on Acronym: H.O.
H.O.	(Haggkvist+Oja)
*****	Avoid the usage of H.O., prefer [HO73]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: 1H
1H	(HEAO A-1 experiment)= (HEAO) = (LASS)
Write:	<<1H HHMM+DDd>>
N:	842
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Sources detected with the NRL Large Area Sky Survey Experiment on the HEAO 1 satellite. First 6 months of data from HEAO 1. limiting flux 250 nJy at 5 keV or about 0.25 UFU. 90per100 complete at flux level 1.5 microJy at 5 keV. Cross-referenced with published literature
Ref:	=1984ApJS...56..507W
by	WOOD K.S. , MEEKINS J.F., YENTIS D.J., SMATHERS H.W., McNUTT D.P., BLEACH R.D., BYRAM E.T., CHUBB T.A., FRIEDMAN H., MEIDAV M.
	Astrophys. J., Suppl. Ser., 56, 507-649 (1984)
	The HEAO A-1 X-ray source catalog.
o	<1H HHMM+DDd> N=842
=E=	Catalogue in electronic form as VII/80 Table 3: (Nos U1-U29), UV excess candidates Table 3: (Nos U1-U29), UV excess candidates Table 3: (Nos U1-U29), UV excess candidates
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [H2000]
[H2000]	(Hawkins, 2000)
Write:	<<[H2000] HHMMSS.ss+DDMMSS.s>>
N:	385
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Ref:	=2000A&AS..143..465H
by	HAWKINS M.R.S.
	Astron. Astrophys., Suppl. Ser., 143, 465-481 (2000)
	Quasar variability: Correlations with amplitude.
o	Appendix: <[H2000] HHMMSS.ss+DDMMSS.s> N=385.
=E=	Catalogue in electronic form as J/A+AS/143/465
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H2001]
[H2001]	(Hunter, 2001)
Write:	<<[H2001] N-N>>
N:	4+2+7
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST observations of IC 10. Search for stellar clusters in CCD PC1, WF2, WF4 (leading 'N' in the format respectively 1, 2, 4).
in source:	IC 10
Ref:	=2001ApJ...559..225H
by	HUNTER D.A.
	Astrophys. J., 559, 225-242 (2001)
	The stellar population and star clusters in the unusual local group galaxy IC 10.
o	Fig.2, Table 2: <[H2001] N-N> (Nos 1-1 to 1-4, 2-1 to 2-2, 4-1 to 4-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H2003]
[H2003]	(Hornoch, 2003)
Write:	<<[H2003] JHHMMSS.ss+DDMMSS.s>>
N:	1+1
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Stat:	is completely incorporated in Simbad
Note:	Lelekovice observations. Discovery of two new novae in M 31.
in source:	M 31 = NGC 224
Ref:	=2003IAUC.8248....2H
by	HORNOCH K.
	IAU Circ., 8248, 2-None (2003)
	Novae in M31.
o	<[H2003] JHHMMSS.ss+DDMMSS.s> N=1.
Ref:	=2003IAUC.8157....4H
by	HORNOCH K.
	IAU Circ., 8157, 4-None (2003)
	Nova in M31.
o	<[H2003] JHHMMSS.ss+DDMMSS.s> N=1 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H2004]
[H2004]	(Hawkins, 2004)= ([H2004a])
Write:	<<[H2004] HHMMSS.ss+DDMMSS.s>>
N:	67
Object:	Seyfert G (SIMBAD class: AGN = Active Galaxy Nucleus)
Stat:	is completely incorporated in Simbad
Note:	Discovery of a new class of AGN: Sey 1 galaxies without broad emission lines.
Ref:	=2004A&A...424..519H
by	HAWKINS M.R.S.
	Astron. Astrophys., 424, 519-529 (2004)
	Naked active galactic nuclei.
o	Table 1: <[H2004] HHMMSS.ss+DDMMSS.s> N=67.
=E=	Catalogue in electronic form as J/A+A/424/519
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H2004a]
[H2004a]	(Hawkins, 2004)
*****	Avoid the usage of [H2004a], prefer [H2004]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H2004b]
[H2004b]	(Hiriart, 2004) (Not yet in Simbad)
Write:	<<[H2004b] A>>
N:	8
Object:	Knot (SIMBAD class: PartofCloud = Part of Cloud)
Note:	Search for molecular Hydrogen distribution in the Ring Nebula.
in source:	NAME Ring Nebula
Ref:	=2004PASP..116.1135H
by	HIRIART D.
	Publ. Astron. Soc. Pac., 116, 1135-1142 (2004)
	Molecular hydrogen kinematics and structure in the Ring Nebula.
o	Table 2: <[H2004b] A> (Nos A-H).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H2005]
[H2005]	(Hojaev, 2005)= ([H2005a])
Write:	<<[H2005] JHHMMSS.ss+DDMMSS.s>>
N:	8
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Optical photometry at the 0.6m and 1.5m telescopes at Mt. Maidakan (Uzbekistan). Spectroscopy at the 2.16m telescope of Bejing University. Young stars in the NGC 6823 - 6820 complex.
in source:	NGC 6823
Ref:	=2005JApA...26..293H
by	HOJAEV A.S.
	J. Astrophys. Astron., 26, 293-299 (2005)
	Collaborative research of open star clusters.
o	Table 2: <[H2005] JHHMMSS.ss+DDMMSS.s> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H2005a]
[H2005a]	(Hojaev, 2005)
*****	Avoid the usage of [H2005a], prefer [H2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H2005b]
[H2005b]	(Halpern, 2005)
Write:	<<[H2005b] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Note:	The optical candidate is later defined as the host galaxy of GRB 050826 in 2006GCN..4749....1H.
Ref:	=2005GCN..3891....1H
by	HALPERN J.P.
	GRB Coordinates Network, Circular Service, 3891, 1-None (2005)
	GRB 050826: optical candidate.
o	<[H2005b] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H2006]
[H2006]	(Hidalgo-Gamez, 2006) (Not yet in Simbad)
Write:	<<[H2006] ESO 245-05 dN>> <<[H2006] ESO 245-05 hN>> <<[H2006] GR 8 adN>> <<[H2006] GR 8 ahN>>
N:	4+3+11+7
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Study of diffuse ionized gas regions (letter d in the format) and HII regions (letter h in the format) in two galaxies.
in source:	ESO 245-5
in source:	GRDG 8
Ref:	=2006AJ....131.2078H
by	HIDALGO-GAMEZ A.M.
	Astron. J., 131, 2078-2088 (2006)
	Diffuse ionized gas in irregular galaxies. I. GR 8 and ESO 245-G05.
o	Table 3: <[H2006] ESO 245-05 dN> (Nos d1-d4), <[H2006] ESO 245-05 hN> (Nos h1-h3). Table 4: <[H2006] GR 8 adN> (Nos ad1-ad2), <[H2006] GR 8 bdN> (Nos bd1-bd3), <[H2006] GR 8 cdN> (Nos cd1-cd2), <[H2006] GR 8 ddN> (Nos dd1-dd2), <[H2006] GR 8 edN> (Nos ed1-ed2), <[H2006] GR 8 ahN> (No. ah1), <[H2006] GR 8 bhN> (Nos bh1-bh2), <[H2006] GR 8 chN> (No. ch1), <[H2006] GR 8 dhN> (No. dh1), <[H2006] GR 8 ehN> (No. eh1), <[H2006] GR 8 fhN> (No. fh1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H2007]
[H2007]	(Harris, 2007)= ([H2007a])
Write:	<<[H2007] mbNN NNNNNN>> <<[H2007] Offset NNNNN>>
N:	258455+13849
Object:	* (SIMBAD class: Star)
Note:	Mosaic II camera on the 4m telescope at the Cerro-Tololo Inter-American Observatory observations, to search for stars in the Magellanic Bridge.
in source:	Magellanic Clouds:Magellanic Bridge = Magellanic Bridge
Ref:	=2007ApJ...658..345H
by	HARRIS J.
	Astrophys. J., 658, 345-357 (2007)
	The Magellanic bridge: the nearest purely tidal stellar population.
o	Table 4: <[H2007] mbNN NNNNNN> N=29119+14406+10116+9045+9679+8211+6769+9535+10588+9934+31849+109204, <[H2007] Offset NNNNN> (Nos 1-13849).
=E=	Catalogue in electronic form as J/ApJ/658/345
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H2007a]
[H2007a]	(Harris, 2007)
*****	Avoid the usage of [H2007a], prefer [H2007]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H2007b]
[H2007b]	(Hovhannessian, 2007) (Not yet in Simbad)
Write:	<<[H2007b] Group R>>
N:	16
Object:	Stellar Group (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Distribution of stars in NGC 1893. See also [KHE2005].
in source:	NGC 1893
Ref:	=2007Ap.....50..194H
by	HOVHANNESSIAN R.K.
	Ap, 50, 194-202 (2007)
	Distribution of Early-Type Stars and Dusty Matter in the Direction of the Stellar Cluster NGC 1893.
o	Table 2: <[H2007b] Group R> (Nos I-XVI). Table 1, col(2): <Cl* NGC 1893 H NNN> (Nos 1-255).
=E=	Catalogue in electronic form as <J/other/Ap/50.194/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H2008]
[H2008]	(Hornoch, 2008)
Write:	<<[H2008] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	Poss. Nova (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Ondrejov 0.65m telescope observations. Discovery of an apparent nova in M 81.
in source:	M 81 = NGC 3031
Ref:	=2008CBET.1281....1H
by	HORNOCH K.
	CBET, 1281, 1 (2008)
	Possible nova in M81.
o	<[H2008] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H2009]
[H2009]	(Humphrey, 2009)
Write:	<<[H2009] NGC NNNN NNN>>
N:	3754
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of N=19 NGC galaxies. Search for globular cluster candidates.
Ref:	=2009ApJ...690..512H
by	HUMPHREY P.J.
	Astrophys. J., 690, 512-525 (2009)
	Low-mass X-ray binaries and globular clusters in early-type galaxies. II. Globular cluster candidates and their mass-metallicity relation.
o	Table 5: <[H2009] NGC NNNN NNN> N=3754.
=E=	Catalogue in electronic form as <J/ApJ/690/512/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H2012]
[H2012]	(Heithausen, 2012)
Write:	<<[H2012] SAMSN>> <<[H2012] NGC3077-TAN>> <<[H2012] M81-OA>>
N:	13
Object:	Dust Cloud (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Herschel SPIRE and Spitzer MIPS observations of the interacting galaxy triplett M81, M82, and NGC3077.
Ref:	=2012A&A...543A..21H
by	HEITHAUSEN A.
	Astron. Astrophys., 543A, 21-21 (2012)
	On the nature of dust clouds in the region towards M 81 and NGC 3077.
o	Table 1 : <[H2012] SAMSN> (Nos 1-9), <[H2012] NGC3077-TAN> (Nos TA1-TA3), <[H2012] M81-OA> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H2013]
[H2013]	(Howarth, 2013)
Write:	<<[H2013] LMCe NNNNA>> <<[H2013] LMCe NNNNW>>
N:	1675
Object:	Poss. Em* (SIMBAD class: Star)
Note:	Compilation of N=1700 Large Magellanic Cloud (LMC) emission-line candidates.
Ref:	=2013A&A...555A.141H
by	HOWARTH I.D.
	Astron. Astrophys., 555A, 141-141 (2013)
	Emission-line stars in the LMC: the Armagh survey and a metacatalogue.
o	Table A.2: <[H2013] LMCe NNNN> N=1654 among (Nos 1-1675), <[H2013] LMCe NNNNA> N=7, [H2013] LMCe NNNNW> N=39.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H2019]
[H2019]	(Hart, 2019)
Write:	<<[H2019] SDSS JHHMMSS.ss+DDMMSS.s system>> <<[H2019] SDSS JHHMMSS.ss+DDMMSS.s source>>
N:	35+35
Object:	Grav. lens system + Grav. lensed image of a G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=35 gravitational lens systems and N=35 gravitationally lensed emition line galaxies, by SDSS luminous red galaxies.
Ref:	=2019AJ....157..221H
by	HART M.
	Astron. J., 157, 221-221 (2019)
	Sky residual correction.
o	Table 1: <[H2019] SDSS JHHMMSS.ss+DDMMSS.s system> N=35, <[H2019] SDSS JHHMMSS.ss+DDMMSS.s source> N=35.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: H21
H21	(Hughes, 2021)
*****	Avoid the usage of H21, prefer [HSS2021]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 22h
22h	(Field centered at 22h)
*****	Avoid the usage of 22h, prefer Gilmore
Origin	of the Acronym: L = Found in the literature
Details on Acronym: H22
H22	(Hughes, 2022)
*****	Avoid the usage of H22, prefer [HSS2023]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [H25]
[H25]	(Hubble, 1925)= (Hubble)
Write:	<<[H25] VNN>> <<[H25] R>>
N:	15+10
Object:	V* + Nebula (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table I: format ' VNN', (Nos V1-V15) Variable *, identical to [K67] VNN (Nos V1-V15) (Brian Skiff 1999). See also [K67] Table III: format 'R' (Nos I-X) N=10 Nebulae.
in source:	NGC 6822
Ref:	=1925ApJ....62..409H
by	HUBBLE E.P.
	Astrophys. J., 62, 409-433 (1925)
	NGC 6822, a remote stellar system.
o	Table I: <[H25] VNN> (Nos V1-V15). Table III: <[H25] R> (Nos I to X).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H26]
[H26]	(Hubble, 1926) (Not yet in Simbad)
Write:	<<[H26] NN>>
N:	2
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Note:	Format AN for N1 and N2 Novae. See also VHK for the V*.
in source:	M 33 = NGC 598
Ref:	=1926ApJ....63..236H
by	HUBBLE E.P.
	Astrophys. J., 63, 236-274 (1926)
	A spiral nebula as a stellar system: Messier 33.
o	[H26] acronym is not used for the V, the numbering is continued in 1975ApJS...29..303V, all V are 'VHK NN' in SIMBAD.
o	<VHK NN> (Nos 1-45). <[H26] AN> (Nos N1, N2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H26]
[H26]	(Hubble, 1926)
*****	Avoid the usage of [H26], prefer VHK
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H29]
[H29]	(Hubble, 1929)
Note:	Tables I, II, III: (Nos 1-50), often quoted VNN in the literature.
*****	Avoid the usage of [H29], prefer BASW
Details on Acronym: [H29]
[H29]	(Hubble, 1929)= (H) = (Hubble)
Write:	<<[H29] NNN>>
N:	100
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Note:	Tables IV, V: Format 'ANN': (N1-N86), 'N' for Nova. Nos 26, 36, 39 are rejected as novae, and the following omitted on the grounds that the preceding unobserved intervals are excessive: Nos 12, 13, 15, 24, 25, 38, 46, 47, 48, 53, and 73.
in source:	M 31 = NGC 224
Ref:	=1929ApJ....69..103H
by	HUBBLE E.
	Astrophys. J., 69, 103-157 (1929)
	A spiral nebula as a stellar system, Messier 31.
o	Tables I, II, III: [H29] VNN use <BASW NN> (Nos 1-50). Tables IV, V: <[H29] ANN> N=63 among (Nos N1-N86).
Ref:	=1931PASP...43..217M
by	MAYALL N.U.
	PASP, 43, 217 (1931)
	Recent novae in the Great Spiral Nebula in Andromeda (M 31).
o	Table 2: <[H29] ANNN> (Nos N87-N100) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: H2O
H2O	(H2O em. source)
*****	Avoid the usage of H2O, prefer GH2O
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: H2O
H2O	(H2O em. source)
Write:	<<H2O HHMM+DD>>
Object:	H2O Maser + MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	Systematic designation. May be either an acronym (with format LLL.ll+BB.bb) or a specificator
Details on Acronym: H2XMM
H2XMM	(High Energy Large Area Survey, XMM-Newton)
====>	Equivalent to: HELLAS2XMM
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [H32]
[H32]	(Hubble, 1932)= (H) = (Hubble)
Write:	<<[H32] NNN>> <<[H32] R>>
N:	139+8
Object:	Neb. Obj. (SIMBAD class: ISM = Interstellar Medium Object)
Stat:	is completely incorporated in Simbad
Note:	Format 'NNN': table I: (Nos 1-140). Format 'R': 8 objects probably associated with NGC 205 nebula (see p. 55, NGC 205 is a faint companion of M 31), written with a roman num. on the plates.. No. 0 is added in 1969ApJS..171...19V by Van Den Bergh.
in source:	M 31 = NGC 224
Ref:	=1932ApJ....76...44H
by	HUBBLE E.
	Astrophys. J., 76, 44-69 (1932)
	Nebulous objects in Messier 31 provisionnally identified as globular clusters.
o	Finding charts
o	<[H32] NNN> N=140. <[H32] R> N=8
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H37]
[H37]	(Holmberg, 1937)= (Ho) = (Holm) = (Holmberg)
Write:	<<[H37] NNN>>
N:	827
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Ref:	=1937AnLun...6....1H
by	HOLMBERG E.
	Ann. Obs. Lund, 6, 1-None (1937)
	A study of double and multiple galaxies, together with inquiries into some general metagalactic problems.
o	Appendix: <[H37] NNN> (Nos 1-827), <[H37] NNNa> N=1854
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [H37]
[H37]	(Holmberg, 1937)= (Ho) = (Holm) = (Holmberg)
Write:	<<[H37] NNNa>>
N:	1854
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Ref:	=1937AnLun...6....1H
by	HOLMBERG E.
	Ann. Obs. Lund, 6, 1-None (1937)
	A study of double and multiple galaxies, together with inquiries into some general metagalactic problems.
o	Appendix: <[H37] NNN> (Nos 1-827), <[H37] NNNa> N=1854
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: H4
H4	(HEAO satellite, 4th experience)
*****	Avoid the usage of H4, prefer H
Details on Acronym: [H53]
[H53]	(Hoffleit, 1953)= (H) = ([H53a]) = (Hf) = (Hoffleit)
Write:	<<[H53] NN>>
N:	63
Object:	Bright N (SIMBAD class: GalNeb = Nebula)
Note:	Among the 63 bright nebulosities, 6 objects are PN (Nos 4, 38, 39, 48, 62, 69), see [Hf]
Ref:	=1953AnHar.119...37H
by	HOFFLEIT D.
	Ann. Astron. Obs. Harvard Coll., 119, 37-None (1953)
	A preliminary survey of nebulosities and associated B-stars in Car.
o	Catalogue: <[H53] NN> (Nos 1-69) among which: <PN Hf NN> N=6 (Nos 4, 38, 39, 48, 62, 69).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H53a]
[H53a]	(Hoffleit, 1953)
*****	Avoid the usage of [H53a], prefer [H53]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H53b]
[H53b]	(Haro, 1953)
Write:	<<[H53b] NNa>>
N:	9
Object:	Nebula (SIMBAD class: ISM = Interstellar Medium Object)
Stat:	is completely incorporated in Simbad
Note:	Peculiar objects in the Orion Nebula region. (Nos 1a-13a), but the same object is seen in several figures with a different numbering, so: 3a = 4a = 9a = 10a = 14a, and 5a = 6a. See also Haro 4-.
in source:	NAME Orion Nebula
Ref:	=1953ApJ...117...73H
by	HARO G.
	Astrophys. J., 117, 73-82 (1953)
	H-α emission stars and peculiar objects in the region of the Orion Nebula.
o	Table 1: <Haro 4-NNN> (Nos 4-1 to 4-255). Table 2: <[H53b] NNa> (Nos 1a-13a).
Details on Acronym: [H56]
[H56]	(Haro, 1956)= (Haro) = (T)
Write:	<<[H56] NN>>
N:	44
Object:	EmG + Blue G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-10) are Em.G, (Nos 11-44) are Blue G.
Ref:	=1956BOTT....2n...8H
by	HARO G.
	Bol. Obs. Tonantz. Tacub., 2, part no 14, 8-18 (1956)
	Nota preliminar sobre galaxias azules con lineas de emision.
o	Tables I, III: <[H56] NN> (Nos 1-44)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [H60]
[H60]	(Hiltner, 1960)= ([H60a]) = (Hiltner)
Write:	<<[H60] a>>
N:	23
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
in source:	M 33 = NGC 598
Ref:	=1960ApJ...131..163H
by	HILTNER W.A.
	Astrophys. J., 131, 163-167 (1960)
	Colors and magnitudes of clusters in M 31 and M 33.
o	Table 2: <[H60] a> N=23
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H60a]
[H60a]	(Hiltner, 1960)
*****	Avoid the usage of [H60a], prefer [H60]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H60b]
[H60b]	(Hodge, 1960)= (Anon) = (H) = (Hodge) = (HodgeC60)
Write:	<<[H60b] NN>>
N:	12
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Note:	Nos 1-14. Nos 12, 13 are missing.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1960ApJ...131..351H
by	HODGE P.W.
	Astrophys. J., 131, 351-357 (1960)
	Studies of the Large Magellanic Cloud. I. The red globular clusters.
o	Table 1: <[H60b] NN> (Nos 1-14) Nos 12, 13 missing
Details on Acronym: [H61]
[H61]	(Hodge, 1961)
Write:	<<[H61] a>> <<[H61] I-N-NNN>> <<[H61] II-NNN>>
N:	20+933+124
Object:	* (SIMBAD class: Star)
Note:	Table 1, Fig.2: N=20 among (Nos a-w) secondary seq. stars. Table 3, Fig.4: field stars in Area I, regions (Nos 1-4), N=933. Table 4, Fig.5: field stars in Area II, N=124.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1961ApJS....6..235H
by	HODGE P.W.
	Astrophys. J., Suppl. Ser., 6, 235-252 (1961)
	Studies of the Large Magellanic Cloud. VI. Properties of 1057 field stars.
o	Table 1, Fig.2: <[H61] a> N=20 among (Nos a-w). Table 3, Fig.4: <[H61] I-N-NNN> N=933. Table 4, Fig.5: <[H61] II-NNN> N=124.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H65]
[H65]	(Hodge, 1965)= (H)
Write:	<<[H65] A>> <<[H65] NNNA>>
N:	14+523
Object:	* (SIMBAD class: Star)
Note:	Table 1: photoelectric standards, format 'A', N=14 among (Nos A-Z). Table 2: stars (Nos 1-523)
in source:	NAME Scl Galaxy
Ref:	=1965ApJ...142.1390H
by	HODGE P.W.
	Astrophys. J., 142, 1390-1397 (1965)
	A color-magnitude diagram for the Sculptor dwarf galaxy.
o	Table 1: <[H65] A> N=14 among (Nos A-Z), Table 2: <[H65] NNNA> N=523
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H68]
[H68]	(Hulsbosch, 1968)= (A) = (AC) = (B) = (C) = (Complex) = (D) = (G) = (GP) = (H) = (K) = (L) = (M) = (P) = (Sh) = (Sm) = (SP) = (WA) = (WB) = (WC) = (WD) = (WE)
Write:	<<[H68] A>> <<[H68] AA>> <<[H68] Aa>> <<[H68] A R>> <<[H68] AA 0>> <<[H68] AA R>>
N:	43
Object:	HVC (SIMBAD class: HVCld = High-velocity Cloud)
Stat:	is completely incorporated in Simbad
Note:	A, AC etc... stand for hydrogen complexes, then subcomponents or clouds are specified as A I, A II, ... See also [GVC73] for : parts of the cloud '[H68] A' ([GVC73] A R.N), parts of the cloud '[H68] C' ([GVC73] C R A), parts of the cloud '[H68] M' ([GVC73] M R.N) and [W2001c] for new cores in '[H68] C'.
in source:	NAME Gal Anticenter
Ref:	=1968BAN....20...33H
by	HULSBOSCH A.N.M.
	Bull. Astron. Inst. Netherlands, 20, 33-39 (1968)
	High-velocity hydrogen complexes at high galactic latitudes.
o	<[H68] A>, <[H68] AC>, <[H68] AC R> (Nos I to III), <[H68] B>, <[H68] C>, <[H68] C R> (Nos I to III), <[H68] K>, <[H68] M>, <[H68] M R> (Nos I to II), <[H68] P>, <[H68] Sh>, <[H68] Sm>, <[H68] SP>
Ref:	=1973A&AS...12..209G
by	GIOVANELLI R. , VERSCHUUR G.L., CRAM T.R.
	Astron. Astrophys., Suppl. Ser., 12, 209-262 (1973)
	High resolution studies of high velocity clouds of neutral hydrogen.
o	Table 8: concentration in OMM 360 (=Ohio MM 360) not in SIMBAD
o	Table 3: <[H68] A R> N=6 (Nos A I to A VI). Table 4: <[GVC73] A R.N> N=9 (Nos A I.1 to A I.4, A II.1 to AII.2, A IV.1 to A IV.3). Table 5, Fig.8: <[GVC73] C R A> N=4 (Nos C I B, C III A to C III C). Table 7: <[GVC73] M R.N> N=6 (Nos I.1 to M I.3, M II.1 to M II.3).
Ref:	=1991A&A...250..509W
by	WAKKER B.P. , VAN WOERDEN H.
	Astron. Astrophys., 250, 509-532 (1991)
	Distribution and origin of high-velocity clouds. III. Clouds, complexes and populations.
o	Table 1: <WV NNN> (Nos 1-561). Table 3: <[H68] A> (Nos D, G, H, L), <[H68] AA> (Nos WA-WD), <NAME GCN Complex>, <NAME GCP Complex>, <NAME ACHV Complex>, <NAME ACVHV Complex>.
Ref:	=1993ApJ...416L..29D
by	DANLY L. , ALBERT C.E., KUNTZ K.D.
	Astrophys. J., 416, 29-32 (1993)
	A determination of the distance to the high-velocity cloud complex M.
o	<[H68] M III> added.
Ref:	=2001ApJS..136..463W
by	WAKKER B.P.
	Astrophys. J., Suppl. Ser., 136, 463-535 (2001)
	Distances and metallicities of high- and intermediate-velocity clouds.
o	probes M15NWcore, M15SEcore and 0159+625 not in Simbad.
o	Table 2, text: <[H68] AA> (Nos CD, GP, WE) added, <[H68] A R> (Nos H I to H III, M IV) added. Table 2, text: <[W2001c] PP Arch> N=1, <[W2001c] Complex gp> N=1. Fig.6, text: <[W2001c] Core CeR> (Nos CeI to CeV), <[W2001c] Core AA> (Nos CD, CK).
=E=	Catalogue in electronic form as J/ApJS/136/463
Details on Acronym: [H69]
[H69]	(Hodge, 1969)= (Ho) = (Hodge)
Write:	<<[H69] NGC NNNN NNN>> <<[H69] Ho R NNN>>
N:	1501
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Table 2: In the format 'NGC NNNN' for the galaxies NGC 628, NGC 925, NGC 1232, NGC 1300, NGC 1365, NGC 1969, NGC 2403, NGC 2903, NGC 3109, NGC 3184, NGC 3359, NGC 3486, NGC 4449, NGC 5068. NGC 5457, NGC 5474, NGC 6822, NGC 6946, NGC 7793, and 'Ho R' for 'Ho II' or 'Ho V' (2 Holmberg galaxies)
Ref:	=1969ApJS...18...73H
by	HODGE P.W.
	Astrophys. J., Suppl. Ser., 18, 73-None (1969)
	H II regions in twenty nearby galaxies.
o	Table 2: <[H69] NGC NNNN NNN> and <[H69] Ho R NNN> N=1501
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H71]
[H71]	(Hulsboch, 1971)
Write:	<<[H71] LLL+B-VVV>>
N:	3
Object:	HVC (SIMBAD class: HVCld = High-velocity Cloud)
Stat:	is completely incorporated in Simbad
Ref:	=1971A&A....14..489H
by	HULSBOSCH A.N.M.
	Astron. Astrophys., 14, 489-492 (1971)
	A distance determination program for some low-latitude high-velocity neutral hydrogen clouds around longitude 125 °.
o	Table 1: <[H71] LLL+B-VVV> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H72]
[H72]	(Harris, 1972)= ([H72a])
Write:	<<[H72] W>> <<[H72] Wa>> <<[H72] Ex>>
N:	6
Object:	Spot (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	3C 390.3 is observed, and several components defined. Table I: N , C, and S, are North, Center, and South components, Ex is an Extended component, Fig.4: Np is the North preceding spot, Sf the South following. See also [D81b]
in source:	3C 390.3
Ref:	=1972MNRAS.158....1H
by	HARRIS A.
	Mon. Not. R. Astron. Soc., 158, 1-11 (1972)
	High resolution observations of 3C 390.3 at 2.7 and 5GHz.
o	Table I: <[H72] W> (Nos N, C, S) N=3, <[H72] Ex> N=1. Fig.4: <[H72] Wa> (Nos Np, Sf) N=2
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H72a]
[H72a]	(Harris, 1972)
*****	Avoid the usage of [H72a], prefer [H72]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H72b]
[H72b]	(Hodge, 1972)= (Dk)
Write:	<<[H72b] NN>>
N:	68
Object:	Dark Nebula (SIMBAD class: DarkNeb = Dark Cloud (nebula))
Note:	See also [H88b]. Identif. charts.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1972PASP...84..365H
by	HODGE P.W.
	Publ. Astron. Soc. Pac., 84, 365-372 (1972)
	Dark nebulae in the Large Magellanic Cloud.
o	Table I: <[H72b] NN> (Nos 1-68).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H73]
[H73]	(Hodge, 1973)= (AR) = (dc) = ([H73a])
Write:	<<[H73] AR NN>>
N:	12
Object:	Cloud (SIMBAD class: Cloud)
Note:	N=12 Absorption Regions (AR) or Dust Clouds (dc) in NGC 205
in source:	NGC 205 = M 110
Ref:	=1973ApJ...182..671H
by	HODGE P.W.
	Astrophys. J., 182, 671-695 (1973)
	The structure and content of NGC 205.
o	Table 10: Sources are <[H32] R' (Nos I-VIII)> in SIMBAD.
o	Table 7: <[H73] AR NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H73a]
[H73a]	(Hodge, 1973) (Not yet in Simbad)
*****	Avoid the usage of [H73a], prefer [H73]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H73b]
[H73b]	(Harris, 1973)
Write:	<<[H73b] A>>
N:	4
Object:	Condensation (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	5 GHz observations at the Cambridge 5-km telescope. N=4 compact components of high density in DR 21. See also [RGG89]
in source:	DR 21
Ref:	=1973MNRAS.162p...5H
by	HARRIS S.
	Mon. Not. R. Astron. Soc., 162, part no 16, 5-10 (1973)
	5GHz observations of small-scale structure in DR21.
o	Fig.1, Table I: <[H73b] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H74]
[H74]	(Hodge, 1974)= ([H74a]) = (HDN)
Write:	<<[H74] NN>>
N:	45
Object:	Dark Cloud (SIMBAD class: DarkNeb = Dark Cloud (nebula))
Stat:	is completely incorporated in Simbad
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1974PASP...86..263H
by	HODGE P.W.
	Publ. Astron. Soc. Pac., 86, 263-266 (1974)
	Dark nebulae in the Small Magellanic Cloud.
o	Table I: <[H74] NN> (Nos 1-45)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H74a]
[H74a]	(Hodge, 1974)
*****	Avoid the usage of [H74a], prefer [H74]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H74b]
[H74b]	(Hodge, 1974)= (H)
Write:	<<[H74b] NGC NNNN NNN>> <<[H74b] Sextans A N>> <<[H74b] Sextans B N>>
N:	869
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	HII regions in the N=18 galaxies listed in Table 1. All the HII regions found in Table 1 are neither listed in Table 2, nor found in the Atlas, but some of them are found later in the literature.
in source:	NGC 520
in source:	NGC 2685
in source:	NGC 2911
in source:	NGC 3351
in source:	NGC 3627
in source:	NGC 4254
in source:	NGC 4303
in source:	NGC 4321
in source:	NGC 4394
in source:	NGC 4548
in source:	NGC 4569
in source:	NGC 5921
in source:	NGC 5964
in source:	NGC 6015
in source:	NGC 6503
in source:	NGC 6643
in source:	Sextans A = DDO 75
in source:	Sextans B = DDO 70
Ref:	=1974ApJS...27..113H
by	HODGE P.W.
	Astrophys. J., Suppl. Ser., 27, 113-119 (1974)
	A second survey of HII regions in galaxies.
o	<[H74b] NGC NNNN NNN>, <[H74b] Sextans A N>, <[H74b] Sextans B N> N=869
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H74c]
[H74c]	(Hargrave, 1974)
Write:	<<[H74c] A>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Cambridge radio telescope is used to map M 82.
in source:	M 82 = NGC 3034
Ref:	=1974MNRAS.168..491H
by	HARGRAVE P.J.
	Mon. Not. R. Astron. Soc., 168, 491-503 (1974)
	Observations of M 82 at 5 GHz with the 5-Lm radio telescope.
o	Table I: <[H74c] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H75]
[H75]	(Hodge, 1975)= (C) = ([H75a])
Write:	<<[H75] NN>>
N:	11
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1975IrAJ...12...77H
by	HODGE P.W.
	Irish Astron. J., 12, 77-81 (1975)
	Clusters of the Magellanic Clouds.
o	Table 4: <[H75] NN> (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H75a]
[H75a]	(Hodge, 1975)
*****	Avoid the usage of [H75a], prefer [H75]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H75b]
[H75b]	(Hulsbosch, 1975)
Write:	<<[H75b] LLL+BB-VVV>> <<[H75b] LLL.l+BB.b-VVV>>
N:	89
Object:	HVC + IVC (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	Identif. charts. See also HVC and IVC
Ref:	=1975A&A....40....1H
by	HULSBOSCH A.N.M.
	Astron. Astrophys., 40, 1-25 (1975)
	Studies on high-velocity clouds of neutral hydrogen.
o	Table 4: <[H75b] LLL+BB-VVV>, <[H75b] LLL.l+BB.b-VVV> N=89.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H76]
[H76]	(Hodge, 1976)= (H) = ([H76a])
Write:	<<[H76] NNNa>>
N:	709+30
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	N=709, (Nos 1-662). (Nos 709-729) are outer HII regions from Schmidt plate. For map, see Hodge 1976ApJS vol. 18 p. 73
in source:	NGC 628 = M 74
Ref:	=1976ApJ...205..728H
by	HODGE P.W.
	Astrophys. J., 205, 728-744 (1976)
	H II regions in NGC 628. I. Positions and sizes.
o	<[H76] NNNa> (Nos 1-662) and (Nos 709-729), N=739
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H76a]
[H76a]	(Hodge, 1976)
*****	Avoid the usage of [H76a], prefer [H76]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H76b]
[H76b]	(Hodge, 1976)
Write:	<<[H76b] N>>
N:	4
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
in source:	NGC 628 = M 74
Ref:	=1976AJ.....81...25H
by	HODGE P.W.
	Astron. J., 81, 25-29 (1976)
	The structure of NGC 147.
o	Table III: <[H76b] N> (Nos 1-4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H77]
[H77]	(Hodge, 1977)= ([H77a]) = (Ho) = (Hodge) = (KH) = (PH)
Write:	<<[H77] A>> <<[H77] Ass NN>> <<[H77] Cl* NN>> <<[H77] HII NN>> <<[H77] Cld NN>>
N:	9+16+35+16+11
Object:	Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	format 'A', N=9 photoelectric standards. format 'Ass NN', N=16 Assoc. . format 'Cl NN', N=35 stellar clusters, (Nos 27-35) added in 2004PASP..116..497K. format 'HII NN', N=16 HII regions, see also [H69]. format 'Cld NN', N=11 dust clouds.
in source:	NGC 6822
Ref:	=1977ApJS...33...69H
by	HODGE P.W.
	Astrophys. J., Suppl. Ser., 33, 69-82 (1977)
	The structure and contents of NGC 6822.
o	Table 2: <[H77] A> (Nos A-K, H missing). Table 8: <[H77] Ass NN> (Nos 1-16). Table 11: <[H77] Cl* NN> (Nos 1-26). Table 13: <[H77] HII NN> (Nos 1-16). Table 14: <[H77] Cld NN> (Nos 1-11).
Ref:	=2004PASP..116..497K
by	KRIENKE K. , HODGE P.
	Publ. Astron. Soc. Pac., 116, 497-505 (2004)
	Newly identified star clusters in NGC 6822, and the age distribution of its cluster system.
o	Table 2: <[H77] Cl* NN> (Nos 27-35) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H77a]
[H77a]	(Hodge, 1977)
*****	Avoid the usage of [H77a], prefer [H77]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H77b]
[H77b]	(Hanes, 1977)
Write:	<<[H77b] NGC NNNN NN>> <<[H77b] NGC NNNN-NNNN NN>> <<[H77b] NGC NNNN-NNNN-NNNN NN>>
N:	960
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	Table 5: representative sequences of 60 objects per programme galaxy, identified on Plates 1 to 16.
in source:	NAME Virgo Cluster
Ref:	=1977MmRAS..84...45H
by	HANES D.A.
	Mem. R. Astron. Soc., 84, 45-60 (1977)
	The luminosity distribution of globular clusters in the Virgo cluster of galaxies.
o	Table 5: <[H77b] NGC NNNN NN>, <[H77b] NGC NNNN-NNNN NN>, <[H77b] NGC NNNN-NNNN-NNNN NN>, N=60x16.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H78]
[H78]	(Hodge, 1978)= ([H78a])
Write:	<<[H78] Ass NN>> <<[H78] Cl* NN>> <<[H78] Cld NN>>
N:	20+43+11
Object:	Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 5: format 'Ass NN', N=20 stellar assoc. in IC 1613. Table 7: format 'Cl* NN', N=43 star cluster candidates in IC 1613. Table 8: format 'Cld NN', N=11 poss. dust clouds in IC 1613. Maps
in source:	IC 1613
Ref:	=1978ApJS...37..145H
by	HODGE P.W.
	Astrophys. J., Suppl. Ser., 37, 145-167 (1978)
	The structure and content of IC 1613.
o	Table 5: <[H78] Ass NN> N=20, Table 7: <[H78] Cl* NN> N=43, Table 8: <[H78] Cld NN> N=11
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H78a]
[H78a]	(Hodge, 1978)
*****	Avoid the usage of [H78a], prefer [H78]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H78b]
[H78b]	(Hulsbosch, 1978)
Write:	<<[H78b] LLL+BB-VVV>>
N:	39
Object:	Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Ref:	=1978A&A....66L...5H
by	HULSBOSCH A.N.M.
	Astron. Astrophys., 66, 5-8 (1978)
	A high sensitivity survey of hydrogen at very high velocities (Preliminary Report).
o	Table 1: <[H78b] LLL+BB-VVV> N=39.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H79]
[H79]	(Hodge, 1979)
Note:	Tab. unpublished in Hodge 1979,
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: H80
H80	(Hodge, 1980)
*****	Avoid the usage of H80, prefer [H80b]
Origin	of the Acronym: L (1999AcA....49..521P)
Details on Acronym: H80
H80	(Hintzen, 1980)
*****	Avoid the usage of H80, prefer [H80c]
Origin	of the Acronym: L (1998AJ....116.1529H)
Details on Acronym: H80-F
H80-F	(Hodge, 1980, Field)
*****	Avoid the usage of H80-F, prefer [H80b]
Origin	of the Acronym: L (1999AJ....117..238B)
Details on Acronym: [H80]
[H80]	(Hodge, 1980)= ([H80a])
Write:	<<[H80] NNN>>
N:	730
Object:	Dark Nebula (SIMBAD class: DarkNeb = Dark Cloud (nebula))
in source:	M 31 = NGC 224
Ref:	=1980AJ.....85..376H
by	HODGE P.W.
	Astron. J., 85, 376-386 (1980)
	The dark nebulae of M 31.
o	<[H80] NNN> N=730
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H80a]
[H80a]	(Hodge, 1980)
*****	Avoid the usage of [H80a], prefer [H80]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H80b]
[H80b]	(Hodge, 1980)= H80 = (H80-F)
Write:	<<[H80b] F-NN>>
N:	41+24+27+7+23
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Cl* in 5 fields 1 to 5, complemented in 1988PASP..100.1051H. S
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1980AJ.....85..423H
by	HODGE P.W.
	Astron. J., 85, 423-431 (1980)
	A 4-m census of faint star clusters in the Large Magellanic Cloud.
o	Table III: <[H80b] 1-NN> (Nos 1-1 to 1-51), <[H80b] 2-NN> (Nos 2-1 to 2-24), <[H80b] 3-NN> (Nos 3-1 to 3-27), <[H80b] 4-N> (Nos 4-1 to 4-7), <[H80b] 5-NN> (Nos 5-1 to 5-23)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H80c]
[H80c]	(Hintzen, 1980)= (H80)
Write:	<<[H80c] AWM7 NNNA>> <<[H80c] ANNNN NNN>>
N:	70
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Fig.1: Finding Charts
in source:	AWM 7
in source:	ACO 1213
in source:	ACO 1795
in source:	ACO 2589
in source:	ACO 2666
Ref:	=1980AJ.....85..626H
by	HINTZEN P.
	Astron. J., 85, 626-636 (1980)
	The use of the Kitt Peak IDS in determing galaxy redshifts: results for five clusters.
o	Table I: <[H80c] AWM7 NNNNA> N=19 among (Nos 1-14)+(Nos 101-107), <[H80c] A1213 NNN> N=10 among (Nos 1-10)+(Nos 102-104), <[H80c] A1795 NNN> N=13 among (Nos 101-140), <[H80c] A2589 NNN> N=14 among (Nos 102-133), <[H80c] A2666 NNN> N=16 among (Nos 3-12)+(Nos 101-106).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H81]
[H81]	(Hodge, 1981)= (C) = [H79] = (HO2)
Write:	<<[H81] B-NNN>>
N:	413
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Note:	1981, Atlas of the Andromeda galaxy, Ed: Univ. of Washington Press. Table B: format 'B-NNN', N=413 OCl from Hodge, 1979. Table A: N=355 GCl use 'SKHB NNN'. Table C: N=188 Stellar Assoc. use '[V64] NNN'. Table D: N=730 dust Clouds use '[H80] NNN'. See SKHB, [V64], [H80].
in source:	M 31 = NGC 224
Auth.:	HODGE P.W.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H82]
[H82]	(Hunter, 1982)
Write:	<<[H82] NGC NNNN NNa>> <<[H82] NGC NNNN N'>> <<[H82] Mrk 35 N>> <<[H82] Haro 22 N>> <<[H82] A 1004+10 N>> <<[H82] NGC NNNN DN>>
N:	117+33
Object:	HII + Dust Cloud (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Tables 3, 7: N=117 HII regions in 15 galaxies. Table 8: N=33 Dust regions in 5 galaxies. Maps in Figs 2, 4.
Ref:	=1982ApJ...260...81H
by	HUNTER D.A.
	Astrophys. J., 260, 81-103 (1982)
	Local properties of star-forming regions in irregular galaxies.
o	Haro 22 = [H56] 22, A 1004+10 = Anon 1004+10.
o	Tables 3, 7: <[H82] NGC NNNN NNa>, <[H82] NGC NNNN N'>, <[H82] Mrk 35 N>, <[H82] Haro 22 N>, <[H82] A 1004+10 N>, N=117. Table 8: <[H82] NGC NNNN DN> N=33.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H83]
[H83]	(Hawkins, 1983)= ([H83a])
Write:	<<[H83] NN>>
N:	88
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Ref:	=1983MNRAS.202..571H
by	HAWKINS M.R.S.
	Mon. Not. R. Astron. Soc., 202, 571-585 (1983)
	Variable extragalactic objects: identification and analysis of a complete sample to B =21.
o	Table 2: <[H83] NN> (Nos 1-88)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H83a]
[H83a]	(Hawkins, 1983)
*****	Avoid the usage of [H83a], prefer [H83]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H83b]
[H83b]	(Hojaev, 1983)= (B) = (SB)
Write:	<<[H83b] BNN>> <<[H83b] SBNN>>
N:	76+87
Object:	Flare * + * (SIMBAD class: Star)
Note:	N=76 Byurakan Flare stars format 'BNN' and N=87 Byurakan Suspected Flare stars format 'SBNN'.
Ref:	=1983IBVS.2412....1H
by	HOJAEV A.S.
	IAU Inform. Bull. Var. Stars, 2412, 1-2 (1983)
	Flare stars in Taurus.
o	Table II: <[H83b] BNN> (Nos B1-B11). Table III: <[H83b] SBNN> (Nos SB1-SB11).
Ref:	=1984IBVS.2635....1H
by	HOJAEV A.S.
	IAU Inform. Bull. Var. Stars, 2635, 1-4 (1984)
	Stellar flares in Taurus.
o	Table II: <[H83b] BNN> (Nos B12-B43). Table III: <[H83b] SBNN> (Nos SB12-SB48).
Ref:	=1984IBVS.2636....1H
by	HOJAEV A.S.
	IAU Inform. Bull. Var. Stars, 2636, 1-4 (1984)
	New flare stars in Taurus.
o	Table II: <[H83b] BNN> (Nos B44-B76). Table III: <[H83b] SBNN> (Nos SB49-SB87).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H84a]
[H84a]	(Hanisch, 1984) (Not yet in Simbad)
Write:	<<[H84a] HHMM+DDd>> <<[H84a] HHMM+DDd.N>> <<[H84a] HHMM+DDda>>
N:	97
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	N=97 radio-sources in 37 WBB groups of G
Ref:	=1984A&A...133..192H
by	HANISCH R.J.
	Astron. Astrophys., 133, 192-204 (1984)
	Westerbork observations of 37 poor clusters of galaxies at 1415 MHz.
o	Table 1: <WBB NBB-NNN> or <WBB SBB-NNN> N=37. Table 3: <[H84a] HHMM+DDd> or <[H84a] HHMM+DDd.N> or <[H84a] HHMM+DDda> N=97
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H84b]
[H84b]	(Hintzen, 1984)
Write:	<<[H84b] HHMM+DDd NN>>
N:	227
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 2: N=227 galaxies or stars in the field of 17 QSO. See also [HBS81]
Ref:	=1984ApJS...55..533H
by	HINTZEN P.
	Astrophys. J., Suppl. Ser., 55, 533-550 (1984)
	Wide-angle radio tail QSOs as members of clusters of galaxies. II. Direct optical observations and spectroscopy of QSO fields.
o	Table 2: <[H84b] HHMM+DDd NN> N=227
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H86]
[H86]	(Hodge, 1986)= ([H86a]) = (HodgeC86)
Write:	<<[H86] NNN>>
N:	213
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Plates
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1986PASP...98.1113H
by	HODGE P.
	Publ. Astron. Soc. Pac., 98, 1113-1122 (1986)
	Clusters of the Small Magellanic Cloud. I. A catalog of 213 new clusters.
o	Table II: <[H86] NNN> (Nos 1-213)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H86a]
[H86a]	(Hodge, 1986)
*****	Avoid the usage of [H86a], prefer [H86]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H86b]
[H86b]	(Hawkins, 1986)= (HA) = (HB) = (MH)
Write:	<<[H86b] ANN>> <<[H86b] BNN>>
N:	41
Object:	(UVX) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	N=11 UVX objects in sample A, (Nos A1-A11). N=37 UVX objects in sample B, (Nos B1-B37). Some cross-id. between the two samples A and B are: A1 = B1, A2 = B2, A3 = B3, A4 = B4, A8 = B5, A9 = B6, A10 = B7, (A8 is erroneously named A7 in Table 2).
Ref:	=1986MNRAS.219..417H
by	HAWKINS M.R.S.
	Mon. Not. R. Astron. Soc., 219, 417-426 (1986)
	On the nature of objects detected as faint long-term variables.
o	Table 2: A8 is erroneously named A7. [H86b] A8 = [H86b] B5
o	Table 2: <[H86b] ANN> and <[H86b] BNN> N=41
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H86c]
[H86c]	(Halbwachs, 1986)
Write:	<<[H86c] N NNN>>
N:	439+66
Object:	(SIMBAD class: = Double or Multiple Star)
Note:	N=439 common proper motion (CPM) systems among AGK 3 stars. In format: 1 for probability of 98.7% of being physical, 2 NNN for probability of 60% of being physical.
Ref:	=1986A&AS...66..131H
by	HALBWACHS J.L.
	Astron. Astrophys., Suppl. Ser., 66, 131-148 (1986)
	Common proper motion stars in the AGK3.
o	Table I: <[H86c] 1 NNN> (Nos 1 1 to 1 326). Table II: <[H86c] 2 NNN> (Nos 2 1 to 2 113).
=E=	Catalogue in electronic form as I/121
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H87]
[H87]	(Hodapp, 1987)
Write:	<<[H87] NN>>
N:	16
Object:	Field * (SIMBAD class: Star)
in source:	NAME Mon R2 GMC
Ref:	=1987A&A...172..304H
by	HODAPP K.-W.
	Astron. Astrophys., 172, 304-310 (1987)
	A polarimetric study of the Mon R2 star-forming region.
o	IRS 1 to 6 = [BEB76] IRS 1 to 6
o	Table 2: <[H87] NN> (Nos 1-16)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: H88
H88	(Hodge, 1988)= ([H88a]) = (Hodge)
Write:	<<H88 NNN>>
N:	390
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	Table III: (Nos 1-390), 255 are new, in 10 fields complementing 1980AJ.....85..423H. See [H80b] Identif. charts
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1988PASP..100.1051H
by	HODGE P.
	Publ. Astron. Soc. Pac., 100, 1051-1070 (1988)
	A catalog of 255 new clusters in the Large Magellanic Cloud.
o	Table III: <H88 NNN> (Nos 1-390)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [H88a]
[H88a]	(Hodge, 1988)
*****	Avoid the usage of [H88a], prefer H88
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H88b]
[H88b]	(Hodge, 1988)
Write:	<<[H88b] NNN>>
Object:	Cloud (SIMBAD class: Cloud)
Note:	Dust clouds in the LMC. See also [H72b].
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1988PASP..100..346H
by	HODGE P.W.
	Publ. Astron. Soc. Pac., 100, 346-357 (1988)
	Dark nebulae in the Large Magellanic Cloud. II. A 4-m survey.
o	Objects CO NN are LMC-CO NN in SIMBAD.
o	Table II: <[H88b] NNN> (Nos 1-146).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H89]
[H89]	(Hughes, 1989)
Write:	<<[H89] WN>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=3 sources (Nos w1-w3) in Cep A West (= GGD 37).
in source:	Cep A:Cep A West = Cep A West
Ref:	=1989AJ.....97.1114H
by	HUGHES V.A.
	Astron. J., 97, 1114-1119 (1989)
	Radio observations of Cepheus A. II. The optical object Cep A West (the HW object).
o	Table II: <[H89] WN> (Nos W1-W3)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: H92
H92	(Hummel+, 1992) (Not yet in Simbad)
*****	Avoid the usage of H92, prefer [HSK92]
Origin	of the Acronym: L (1999A&A...348..381R)
Details on Acronym: H92
H92	(Harris+, 1992)
*****	Avoid the usage of H92, prefer [HGH92]
Origin	of the Acronym: L (1996ApJ...467..221M)
Details on Acronym: [H92]
[H92]	(Henning, 1992)= (HenG)
Write:	<<[H92] NN>>
N:	39
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Ref:	=1992ApJS...78..365H
by	HENNING P.A.
	Astrophys. J., Suppl. Ser., 78, 365-390 (1992)
	A study of a 21 centimeter-selected sample of galaxies. I. The survey.
o	Table 1: <[H92] NN> (Nos 1-39)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: H93
H93	(Hill+)
*****	Avoid the usage of H93, prefer [HBC93]
Origin	of the Acronym: L (2000AJ....119..787G)
Details on Acronym: [H95]
[H95]	(Higdon, 1995)= (CW)
Write:	<<[H95] NN>> <<[H95] GN>>
N:	29+3
Object:	HII region complex (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Table 2 and Fig. 2: N=29 HII region complexes, (Nos 1-29). Table 3 and Fig. 1: N=3 Galaxies, (Nos G1-G3).
in source:	NAME Cartwheel Galaxy
Ref:	=1995ApJ...455..524H
by	HIGDON J.L.
	Astrophys. J., 455, 524-535 (1995)
	Wheels of fire. I. Massive star formation in the Cartwheel ring galaxy.
o	Table 2: <[H95] NN> (Nos 1-29), Table 3: <[H95] GN> (Nos G1-G3)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H96]
[H96]	(Henden, 1996)
Write:	<<[H96] VNNNN CCC NN>> <<[H96] AA CCC NNA>>
N:	621
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 3: Comparison stars, for all * of table 2
Ref:	=1996AJ....111..902H
by	HENDEN A.A.
	Astron. J., 111, 902-912 (1996)
	Faint Cepheid studies. I. Comparison with existing data sets.
o	Table 3: <[H96] VNNNN CCC NN>, <[H96] AA CCC NN> N=335
Ref:	=1996AJ....112.2757H
by	HENDEN A.A.
	Astron. J., 112, 2757-2768 (1996)
	Faint cepheid studies. II. Stars with published periods.
o	Table 3: <[H96] VNNNN CCC NN>, <[H96] AA CCC NN> N=293
=E=	Catalogue in electronic form as J/AJ/111/902
=E=	Catalogue in electronic form as J/AJ/112/2757
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H97]
[H97]	(Hjellming, 1997)= ([H97a])
Write:	<<[H97] A>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	3 candidate radio-sources, 2 inside and 1 on the edge of the error box region of XTE J1739-302. [H97] B = XTE J1739-302
Ref:	=1997IAUC.6750S...1H
by	HJELLMING R.M.
	IAU Circ., 6750, 1-None (1997)
	XTE J1739-302.
o	<[H97] A> (Nos A-C)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H97a]
[H97a]	(Hjellming, 1997)
*****	Avoid the usage of [H97a], prefer [H97]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H97b]
[H97b]	(Hillenbrand, 1997)
Write:	<<[H97b] NNNNa>> <<[H97b] NNNNN>>
N:	1576+829+1668
Object:	* (SIMBAD class: Star)
Note:	(Nos 1-1053) are identical to JW NNNN. 34 stars with a numbering between (Nos 1054-2999) are identical to Parenago NNNN. (Nos 9000-9326) (= 9NNN) are identical to PSH NNN. Nos among (Nos 10003-11115) are added in 2002A&A...396..513H.
in source:	NAME ONC
Ref:	=1997AJ....113.1733H
by	HILLENBRAND L.A.
	Astron. J., 113, 1733-1768 (1997)
	On the stellar population and star-forming history of the Orion Nebula Cluster.
o	Tables 1, 3: <[H97b] NNNNa> N=1576 among (Nos 1-9326).
Ref:	=2002A&A...396..513H
by	HERBST W. , BAILER-JONES C.A.L., MUNDT R., MEISENHEIMER K., WACKERMANN R.
	Astron. Astrophys., 396, 513-532 (2002)
	Stellar rotation and variability in the Orion Nebula Cluster.
o	Table 1: <[H97b] NNNNN> N=829 among (Nos 10003-11115) added.
Ref:	=2009A&A...502..883R
by	RODRIGUEZ-LEDESMA M.V. , MUNDT R., EISLOEFFEL J.
	Astron. Astrophys., 502, 883-904 (2009)
	Rotational studies in the Orion nebula cluster: from solar mass stars to brown dwarfs.
o	Table 1: <[H97b] NNNNN> N=1668 among (Nos 20000-21668).
=E=	Catalogue in electronic form as J/AJ/113/1733
=E=	Catalogue in electronic form as J/A+A/502/883
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H98]
[H98]	(Hojaev, 1998)= ([H98a])
Write:	<<[H98] BH-a NN>> <<[H98] SBH-a NN>>
N:	20+18
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=20 Byurakan H-alpha emission stars, format 'BH-a NN'. Table 3: N=18 Byurakan Suspected H-alpha emission stars, format 'SBH-a NN'
Ref:	=1998PASA...15..152H
by	HOJAEV A.S.
	Publications - Astron. Soc. Australia, 15, 152-154 (1998)
	Some results of an H-α survey in the Taurus dark clouds.
o	objects B41, B4, SB33 = [H83b] B41, B4, SB33. object BV5 not found.
o	Table 2: <[H98] BH-a NN> (Nos 1-20). Table 3: <[H98] SBH-a NN> (Nos 1-18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H98a]
[H98a]	(Hojaev, 1998)
*****	Avoid the usage of [H98a], prefer [H98]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H98b]
[H98b]	(Hodapp, 1998)
Write:	<<[H98b] HH 119 IR N>>
N:	5
Object:	(IR) Knot (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	N=5 IR H2 emission knots in HH 119. See also ref. 1992A&A...256..225R for optical knots (HH 119A-C in SIMBAD) and [GO2007b].
in source:	HH 119
Ref:	=1998ApJ...500L.183H
by	HODAPP K.
	Astrophys. J., 500, 183-188 (1998)
	The protostar in B335: near-infrared observations of the class 0 outflow.
o	Optical knots = HH 119A-C in SIMBAD. p. 183: bright star = EQ 1934+0727.
o	Table 1: <[H98b] HH 119 IR N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H98c]
[H98c]	(Hutchings, 1998)
Write:	<<[H98c] N>>
N:	6
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST STIS observations. N=6 brightest companions to the QSO 1345+584.
Ref:	=1998AJ....116...20H
by	HUTCHINGS J.B.
	Astron. J., 116, 20-25 (1998)
	Hubble space telescope resolved image and spectra of the z ≃ 2 QSO 1345+584.
o	Fig.1, Table 2: <[H98c] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H98d]
[H98d]	(Hawkins, 1998)
Write:	<<[H98d] HHMM+DDd>>
N:	5
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Ref:	=1998A&A...340L..23H
by	HAWKINS M.R.S.
	Astron. Astrophys., 340, 23-26 (1998)
	Caustic crossings in quasar light curves?
o	Figs 1-3: <[H98d] HHMM+DDd> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H99]
[H99]	(Hopp, 1999)= ([H99a])
Write:	<<[H99] A>> <<[H99] NNN>>
N:	3+209
Object:	* (SIMBAD class: Star)
Note:	Fig.1: (Nos A-C) are 3 very bright stars in the field of UGC 685. Table 3: N=209 stars in the field of UGC 685.
in source:	UGC 685
Ref:	=1999A&AS..134..317H
by	HOPP U.
	Astron. Astrophys., Suppl. Ser., 134, 317-326 (1999)
	Distance, structure and bright stellar content of the dwarf irregular galaxy UGC 685.
o	Fig.1: <[H99] A> (Nos A-C). Table 3: <[H99] NNN> N=209 among (Nos 12-499).
=E=	Catalogue in electronic form as <J/A+AS/134/317/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H99a]
[H99a]	(Hopp, 1999)
*****	Avoid the usage of [H99a], prefer [H99]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H99b]
[H99b]	(Heithausen, 1999) (Not yet in Simbad)
Write:	<<[H99b] CS A>>
N:	3
Object:	Condensation (SIMBAD class: PartofCloud = Part of Cloud)
Note:	N=3 CS dense condensations in the molecular cloud Gal 123.5+24.9.
in source:	GAL 123.5+24.9
Ref:	=1999A&A...349L..53H
by	HEITHAUSEN A.
	Astron. Astrophys., 349, 53-56 (1999)
	Evidence for inward motion in a galactic cirrus core.
o	MCLD 123.5+24.9 = GAL 123.5+24.9 in SIMBAD
o	Fig.1: <[H99b] CS A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [H99c]
[H99c]	(Han, 1999)= (DD) (Not yet in Simbad)
Write:	<<[H99c] A>>
N:	10
Object:	(SIMBAD class: = Double or Multiple Star)
Note:	N=10 Double Degenerates (DD for the authors).
Ref:	=1999ChA&A..23...75H
by	HAN Z.-W.
	Chinese Astron., 23, 75-88 (1999)
	Channels for the formation of double ° and a Monte-Carlo analysis.
o	Table 1: object 'a' = L 870-2.
o	Table 1: <[H99c] A> (Nos A-J).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HA
HA	(H. Arp)
*****	Avoid the usage of HA, prefer [A72b]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: Ha
Ha	(Haffner)
*****	Avoid the usage of Ha, prefer Haffner
Details on Acronym: HA
HA	(Hawkins, sample A)
*****	Avoid the usage of HA, prefer [H86b]
Origin	of the Acronym: L (Veron)
Details on Acronym: Ha
Ha	(Harvard)
*****	Avoid the usage of Ha, prefer SA
Origin	of the Acronym: L (1969LowOB...7...98P)
Details on Acronym: HA19
HA19	(H. Andrews, 2019)
Write:	<<HA19 NN>> <<HA19 -NN>> (not recognised by Simbad, but found in literature)
N:	53
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ATCA 5.5 and 9GHz observations of N=53 in the field of radio sources the Galactic cluster Westerlund 1.
in source:	Cl Westerlund 1
Ref:	=2019A&A...632A..38A
by	ANDREWS H. , FENECH D., PRINJA R.K., CLARK J.S., HINDSON L.
	Astron. Astrophys., 632A, 38-38 (2019)
	A radio census of the massive stellar cluster Westerlund 1.
o	Table A.4: <HA19 NN> (Nos 3-94).
o	IRS 7 and W1243 not identified.
=E=	Catalogue in electronic form as <J/A+A/632/A38/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HA2001]
[HA2001]	(Hurst+Armstrong, 2001)
Write:	<<[HA2001] JHHMMSS.s+DDMMSS>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of SN 2001IQ.
Ref:	=2001IAUC.7780....2H
by	HURST G.M. , ARMSTRONG M.
	IAU Circ., 7780, 2-None (2001)
	Supernova 2001iq in anonymous galaxy.
o	<[HA2001] JHHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HA2005]
[HA2005]	(Homeier+Alves, 2005)
Write:	<<[HA2005] JHHMMSS.ss+DDMMSS.s>>
N:	25
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	NTT SOFI photometry of W 49 molecular cloud: Candidate stars associated with HII regions in W 49.
in source:	W 49
Ref:	=2005A&A...430..481H
by	HOMEIER N.L. , ALVES J.
	Astron. Astrophys., 430, 481-489 (2005)
	Massive star formation in the W 49 giant molecular cloud: Implications for the formation of massive star clusters.
o	Table 1: <[HA2005] JHHMMSS.ss+DDMMSS.s> N=25.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HA86]
[HA86]	(Hoessel+Anderson, 1986) (Not yet in Simbad)
Write:	<<[HA86] N-NNN>>
N:	3880
Object:	* (SIMBAD class: Star)
Note:	* in NGC 6822 galaxy, format 'N-NNN' where the first digit 'N' stands for a field number (Nos 1-9). See also: [HM82], [HSD83], [HD83], [HD84]
in source:	NGC 6822
Ref:	=1986ApJS...60..507H
by	HOESSEL J.G. , ANDERSON N.
	Astrophys. J., Suppl. Ser., 60, 507-542 (1986)
	Photometry of resolved galaxies. V. NGC 6822.
o	Tables 1-9: objects are not in SIMBAD
o	Table 1: <[HA86] 1-NNN> (Nos 100-459), Table 2: <[HA86] 2-NNN> (Nos 100-348), Table 3: <[HA86] 3-NNN> (Nos 100-520), Table 4: <[HA86] 4-NNN> (Nos 100-559), Table 5: <[HA86] 5-NNN> (Nos 100-726), Table 6: <[HA86] 6-NNN> (Nos 100-504), Table 7: <[HA86] 7-NNN> (Nos 100-446), Table 8: <[HA86] 8-NNN> (Nos 100-575), Table 9: <[HA86] 9-NNN> (Nos 100-535)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HAB2004]
[HAB2004]	(Hagele+Albalacete Colombo+Barba+, 2004)
Write:	<<[HAB2004] NN>>
N:	16
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	2MASS photometry of stars located in the southern part of the Carina Nebula observed with MSX. in the Carina Nebula.
in source:	Carina Nebula = NGC 3372
Ref:	=2004MNRAS.355.1237H
by	HAGELE G.F. , ALBACETE COLOMBO J.F., BARBA R.H., BOSCH G.L.
	Mon. Not. R. Astron. Soc., 355, 1237-1243 (2004)
	G287.84-0.82: an infrared star cluster in the Carina nebula.
o	Table 1: <[HAB2004] NN> (Nos 1-16).
=E=	Catalogue in electronic form as J/MNRAS/355/1237
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HAB84]
[HAB84]	(Hyland+Allen+Barnes+, 1984)
Write:	<<[HAB84] NN>>
N:	88
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
in source:	NAME Orion Nebula
Ref:	=1984MNRAS.206..465H
by	HYLAND A.R. , ALLEN D.A., BARNES P.J., WARD M.J.
	Mon. Not. R. Astron. Soc., 206, 465-474 (1984)
	The distribution and nature of the 2 µ-m radiation of the inner Orion Nebula.
o	Table 1: <[HAB84] NN> (Nos 1-88)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HAC2010]
[HAC2010]	(Heinke+Altamirano+Cohn+, 2010)
Write:	<<[HAC2010] NGC 6440 X-2>>
N:	1
Object:	LMXB (SIMBAD class: LowMassXBin = Low Mass X-ray Binary)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS, RXTE PCA, and Swift XRT observations of a new transient low-mass X-ray binary in the globular cluster NGC 6440.
in source:	NGC 6440
Ref:	=2010ApJ...714..894H
by	HEINKE C.O. , ALTAMIRANO D., COHN H.N., LUGGER P.M., BUDAC S.A., SERVILLAT M., LINARES M., STROHMAYER T.E., MARKWARDT C.B., WIJNANDS R., SWANK J.H., KNIGGE C., BAILYN C., GRINDLAY J.E.
	Astrophys. J., 714, 894-903 (2010)
	Discovery of a second transient low-mass X-ray binary in the globular cluster NGC 6440.
o	<[HAC2010] NGC 6440 X-2> N=1 = <CXOGlb JHHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Had
Had	(Haseda)
Write:	<<Had VNNN>>
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Variable stars from a unpublished list of Haseda K. Objects are found in the name-lists of variable stars published in IBVS. N=2 first references with 'Had VNNN' objects.
Ref:	=2001IBVS.5135....1K
by	KAZAROVETS E.V. , SAMUS N.N., DURLEVICH O.V.
	IAU Inform. Bull. Var. Stars, 5135, 1-None (2001)
	The 76th name-list of variable stars.
o	Table 1: <Had VNN> N=18 among (Nos V16-V57). Table 1: <Mis VNNN> N=65 among (Nos V503-V912).
Ref:	=2003IBVS.5422....1K
by	KAZAROVETS E.V. , KIREEVA N.N., SAMUS N.N., DURLEVICH O.V.
	IAU Inform. Bull. Var. Stars, 5422, 1-None (2003)
	The 77th name-list of variable stars.
o	= 2003BAVSR..52..155
o	Table 2: <Had VNNN> N=35 among (Nos V61-V105), <Mis VNNNN> N=29 among (Nos V952-V1181).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HAD2004]
[HAD2004]	(Herbig+Andrewa+Dahm, 2004)
Write:	<<[HAD2004] NGC 1579 NNN>> <<[HAD2004] LDN 1482 A>>
N:	325+8
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Optical and NIR photometry from University of Hawaii 2.2m telescope observations. Spectroscopy from GMOS at the 8m Gemini North telescope. N=235 stars in NGC 1579. N=8 bright stars in LDN 1482.
in source:	NGC 1579
in source:	LDN 1482
Ref:	=2004AJ....128.1233H
by	HERBIG G.H. , ANDREWS S.M., DAHM S.E.
	Astron. J., 128, 1233-1253 (2004)
	LkHα 101 and the young cluster in NGC 1579.
o	Table 1: <[HAD2004] NGC 1579 NNN> (Nos 1-325). Table 4: <[HAD2004] LDN 1482 A> (Nos A-H). Table 2: <IfAHA NNN> (Nos 187-222) added.
=E=	Catalogue in electronic form as J/AJ/128/1233
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HAE
HAE	(Hα emitter) (Not yet in Simbad)
*****	Avoid the usage of HAE, prefer [TDK2011]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HAE2008]
[HAE2008]	(Heiner+Allen+Emonts+, 2008)
Write:	<<[HAE2008] NNa>>
N:	27+56
Object:	PDR + HI (SIMBAD class: Region = Region defined in the Sky)
Note:	Use of archival GALEX and THINGS HI data to search for Photo Dissociation Regions (PDR) in M 81.
in source:	M 81 = NGC 3031
Ref:	=2008ApJ...673..798H
by	HEINER J.S. , ALLEN R.J., EMONTS B.H.C., VAN DER KRUIT P.C.
	Astrophys. J., 673, 798-809 (2008)
	The volume densities of giant molecular clouds in M81.
o	Table 1: <[HAE2008] NN> (Nos 1-27). Table 2: <[HAE2008] NNa> N=56.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HAE2018]
[HAE2018]	(Hunter+Adamo+Elmegreen+, 2018)
Write:	<<[HAE2018] DDO NN NN>> <<[HAE2018] NGC 3738 N>> <<[HAE2018] Haro 29 N>>
N:	44
Object:	Assoc. (SIMBAD class: Association = Association of Stars)
Note:	HST WFC3 and ACS observations of N=44 OB associations in N=5 galaxies.
in source:	DDO 50
in source:	DDO 53
in source:	DDO 63
in source:	NGC 3738
in source:	[H56] 29
Ref:	=2018AJ....156...21H
by	HUNTER D.A. , ADAMO A., ELMEGREEN B.G., GALLARDO S., LEE J.C., COOK D.O., THILKER D., KAYITESI B., KIM H., KAHRE L., UBEDA L., BRIGHT S.N., RYON J.E., CALZETTI D., TOSI M., GRASHA K., MESSA M., FUMAGALLI M., DALE D.A., SABBI E., CIGNONI M., SMITH L.J., GOULIERMIS D.M., GREBEL E.K., ALOISI A., WHITMORE B.C., CHANDAR R., JOHNSON K.E.
	Astron. J., 156, 21-21 (2018)
	A comparison of young star properties with local galactic environment for LEGUS/LITTLE THINGS dwarf irregular galaxies.
o	Table 3: <[HAE2018] DDO NN NN> N=17+11+6, <[HAE2018] NGC 3738 N> (Nos 1-3), <[HAE2018] Haro 29 N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Haffner
Haffner	(Haffner)= (Ha)
Write:	<<Cl Haffner NNA>>
N:	26
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Stat:	is completely incorporated in Simbad
Note:	Table 1: (Nos 1-22), No. 18 been divided into 18A to 18C. Table 1: Nos (1) to (5) not used in SIMBAD, but Alter and Ruprecht have transformed No. (1) into Haffner 23, and Nos (3) to (5) into Haffner 24 to 26.
Ref:	=1957ZA.....43...89H
by	HAFFNER H.
	Zeitschr. Astrophys., 43, 89-94 (1957)
	Neue galaktische Sternhaufen in der sudlichen Milchstrasse.
o	Table 1: <Cl Haffner NNa> (Nos 1-17, 18A-18C, 19-22), No. (1) is <Cl Haffner 23>, Nos (3) to (5) are respectively <Cl Haffner 24>, <Cl Haffner 25>, <Cl Haffner 26>.
Details on Acronym: HAG
HAG	(HLA ACS Grism)
Write:	<<HAG JHHMMSS.ss+DDMMSS.s>>
N:	54
Object:	G (SIMBAD class: Galaxy)
Note:	Hubble Legacy Archive (HLA) ACS Grism data on N=54 objects in 153 archival fields (or associations). See http://hla.stsci.edu/
Ref:	=2011A&A...530A..86K
by	KUEMMEL M. , ROSATI P., FOSBURY R., HAASE J., HOOK R.N., KUNTSCHNER H., LOMBARDI M., MICOL A., NILSSON K.K., STOEHR F., WALSH J.R.
	Astron. Astrophys., 530A, 86-86 (2011)
	The Hubble Legacy Archive ACS grism data.
o	Table A.2: <HAG JHHMMSS.ss+DDMMSS.s> N=54.
=E=	Catalogue in electronic form as J/A+A/530/A86
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HAG2022]
[HAG2022]	(Hartke+Arnaboldi+Gerhard+, 2022)
Write:	<<[HAG2022] M105-SCAM-NNN>> <<[HAG2022] M105-WWNNN>>
N:	2+18+11+13
Object:	Poss. PN + PN (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Subaru Suprime-Cam observations of N=226 PN candidates in M 105, presented in Hartke et al. 2020A&A...642A..46H. WHT PN.S observations of N=44 additional PNe in M 105, as part of the extremely extended PN.S ETG survey. See also PNS.EPN.
in source:	NAME M 96 GROUP = LEO I GROUP
in source:	NGC 3379 = M 105
Ref:	=2022A&A...663A..12H
by	HARTKE J. , ARNABOLDI M., GERHARD O., COCCATO L., MERRIFIELD M., KUIJKEN K., PULSONI C., AGNELLO A., BHATTACHARYA S., SPINIELLO C., CORTESI A., FREEMAN K.C., NAPOLITANO N.R., ROMANOWSKY A.J.
	Astron. Astrophys., 663A, 12-12 (2022)
	The halo of M 105 and its group environment as traced by planetary nebula populations. II. Using kinematics of single stars to unveil the presence of intragroup light around the Leo I galaxies NGC 3384 and M 105.
o	Table A.1: <[HAG2022] M105-SCAM-NNN> (Nos 001-226). Table A.2: <[HAG2022] M105-NNNN> (Nos N002-N003), <[HAG2022] M105-SNNN> (Nos S001-S018), <[HAG2022] M105-SWNNN> (Nos SW001-SW011), <[HAG2022] M105-WNNN> N=13 among (Nos W001-W014).
=E=	Catalogue in electronic form as <J/A+A/663/A12/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [HAJ2020]
[HAJ2020]	(Hernandez+Aloisi+James+, 2020) (Not yet in Simbad)
Write:	<<[HAJ2020] I Zw 18>> <<[HAJ2020] SBS HHMM-DDd>> <<[HAJ2020] NGC NNNN>> <<[HAJ2020] NGC 5253-N>> <<[HAJ2020] M83-N>>
N:	1+2+4+2+2
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST COS observations of N=11 UV bright sources (young stellar clusters) in nine star-forming galaxies.
Ref:	=2020ApJ...892...19H
by	HERNANDEZ S. , ALOISI A., JAMES B.L., FERLAND G.J., FOX A.J., TOSI M., TUMLINSON J.
	Astrophys. J., 892, 19-19 (2020)
	Newly improved ionization corrections for the neutral interstellar medium: enabling accurate abundance determinations in star-forming galaxies throughout the Universe.
o	Fig. 1, Table 2: <[HAJ2020] I Zw 18> N=1, <[HAJ2020] SBS HHMM+DDd> (Nos SBS 0335-052, SBS 1415+437), <[HAJ2020] NGC NNNN> (Nos NGC 4214, NGC 4670, NGC 4449, NGC 3690), <[HAJ2020] NGC 5253-N> (Nos NGC 5253-1, NGC 5253-2), <[HAJ2020] M83-N> (Nos M83-1, M83-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HAL2011]
[HAL2011]	(Haan+Armus+Laine+, 2011)
Write:	<<[HAL2011] NGC NNNN W>> <<[HAL2011] NGC 6621 Middle>>
N:	10
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRS observations of N=10 galaxies in eight major merger systems.
Ref:	=2011ApJS..197...27H
by	HAAN S. , ARMUS L., LAINE S., CHARMANDARIS V., SMITH J.D., SCHWEIZER F., BRANDL B., EVANS A.S., SURACE J.A., DIAZ-SANTOS T., BEIRAO P., MURPHY E.J., STIERWALT S., HIBBARD J.E., YUN M., JARRETT T.H.
	Astrophys. J., Suppl. Ser., 197, 27 (2011)
	Spitzer IRS spectral mapping of the Toomre sequence: spatial variations of PAH, gas, and dust properties in nearby major mergers.
o	Table 2: <[HAL2011] NGC NNNN W> N=9, <[HAL2011] NGC 6621 Middle> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HaloSat
HaloSat	(X-ray source measured by HaloSat satellite)
Write:	<<HaloSat JHHMM+DDMM>>
N:	about 300 (SIMBAD class: X = X-ray Source)
Note:	HaloSat is a CubeSat-based X-ray observatory sensitive in the soft X-ray band and currently conducting an all-sky survey. http://halosat.physics.uiowa.edu/
Ref:	=2019ApJ...884..162K
by	KAARET P. , ZAJCZYK A., LAROCCA D.M., RINGUETTE R., BLUEM J., FUELBERTH W., GULICK H., JAHODA K., JOHNSON T.E., KIRCHNER D.L., KOUTROUMPA D., KUNTZ K.D., McCURDY R., MILES D.M., ROBISON W.T., SILICH E.M.
	Astrophys. J., 884, 162-162 (2019)
	HaloSat: a CubeSat to study the hot galactic halo.
o	Table 5: <HaloSat JHHMM+DDMM> N=254. University of Iowa
=E=	Catalogue in electronic form as <J/ApJ/884/162/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: Halpha
Halpha	(H-alpha)
*****	Avoid the usage of Halpha, prefer [MR81]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Halpha
Halpha	(H-alpha)
*****	Avoid the usage of Halpha, prefer WSB
Origin	of the Acronym: L (2005A&A...437..611R)
Details on Acronym: [HAM2003]
[HAM2003]	(Heike+Awaki+Misaop+, 2003) (Not yet in Simbad)
Write:	<<[HAM2003] N>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observation of NGC 1569.
in source:	NGC 1569
Ref:	=2003ApJ...591L..99H
by	HEIKE K. , AWAKI H., MISAO Y., HAYASHIDA K., WEAVER K.A.
	Astrophys. J., 591, 99-102 (2003)
	Discovery of bright variable X-ray sources in NGC 1569 with Chandra.
o	Fig.4: <[HAM2003] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HAM2010]
[HAM2010]	(Howell+Armus+Mazzarella+, 2010)= (GOALS)
Write:	<<[HAM2010] GOALS JHHMMSS.s+DDMMSS>>
N:	8
Object:	Pair of G (SIMBAD class: PairG = Pair of Galaxies)
Note:	N=8 systems of galaxies, part of the Great Observatories All-sky LIRG Survey (GOALS). Use of GALEX and Spitzer data.
Ref:	=2010ApJ...715..572H
by	HOWELL J.H. , ARMUS L., MAZZARELLA J.M., EVANS A.S., SURACE J.A., SANDERS D.B., PETRIC A., APPLETON P., BOTHUN G., BRIDGE C., CHAN B.H.P., CHARMANDARIS V., FRAYER D.T., HAAN S., INAMI H., KIM D.-C., LORD S., MADORE B.F., MELBOURNE J., SCHULZ B., U V., VAVILKIN T., VEILLEUX S., XU K.
	Astrophys. J., 715, 572-588 (2010)
	The Great Observatories All-sky LIRG Survey: comparison of ultraviolet and far-infrared properties.
o	Table 2: <[HAM2010] GOALS JHHMMSS.s+DDMMSS> N=8.
=E=	Catalogue in electronic form as <J/ApJ/715/572/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Hanes
Hanes	(Hanes)
Write:	<<Hanes R-NNN>>
Object:	Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Hanes thesis, 1971: In the format 'R-NNN', the roman number stands for quadrants I to IV. Some of these objects are found in 1981ApJ...245..416S, Table 4.
in source:	M 87 = NGC 4486 = Virgo A
Auth.:	HANES D.A.
Origin	of the Acronym: L (1981ApJ...245..416S)
Details on Acronym: [HAP2004]
[HAP2004]	(Hatzidimitriou+Antoniou+Papadakis+, 2004) (Not yet in Simbad)
Write:	<<[HAP2004] NNNN>>
N:	3894
Object:	* (SIMBAD class: Star)
Note:	Skinakas Observatory 1.3m telescope photometric observations
in source:	M 56 = NGC 6779
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HAR2010]
[HAR2010]	(Hagele+Ascasibar+Richards+, 2010)
Write:	<<[HAR2010] NN>>
N:	23
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	MERLIN 1.42GHz observations of NGC 3351.
in source:	NGC 3351
Ref:	=2010MNRAS.406.1675H
by	HAGELE G.F. , ASCASIBAR Y., RICHARDS A.M.S., CARDACI M.V., VASQUEZ J., DIAZ A.I., ROSA GONZALEZ D., TERLEVICH R., TERLEVICH E.
	Mon. Not. R. Astron. Soc., 406, 1675-1686 (2010)
	Subarcsecond radio continuum mapping in and around the spiral galaxy NGC3351 using MERLIN.
o	Table 1: <[HAR2010] NN> (Nos 1-23).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Haro
Haro	(Haro)
*****	Avoid the usage of Haro, prefer [H53b]
Details on Acronym: Haro
Haro	(Haro)
*****	Avoid the usage of Haro, prefer [H56]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Haro
Haro	(Haro)= (Haro 1-)
Write:	<<Haro 1-NN>>
N:	17
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Ref:	=1949AJ.....54..188H
by	HARO G.
	Astron. J., 54, 188-189 (1949)
	Faint spectra showing Hα in emission in the obscuring clouds of Ophiuchus and Scorpius and in a region in Sagittarius.
o	Table I: <Haro 1-NN> (Nos 1-1 to 1-17).
Details on Acronym: Haro
Haro	(Haro)= (Haro 4-)
Write:	<<Haro 4-NNN>>
N:	495
Object:	Em. Obj. (SIMBAD class: EmLine* = Emission-line Star)
Note:	Identif charts. See also [H53b].
in source:	NAME Orion Nebula
Ref:	=1953ApJ...117...73H
by	HARO G.
	Astrophys. J., 117, 73-82 (1953)
	H-α emission stars and peculiar objects in the region of the Orion Nebula.
o	Table 1: <Haro 4-NNN> (Nos 4-1 to 4-255). Table 2: <[H53b] NNa> (Nos 1a-13a).
Ref:	=1982BITon...3...69P
by	PARSAMIAN E.S. , CHAVIRA E.
	Bol. Inst. Tonantzintla, 3, 69-96 (1982)
	Catalog of H-α emission stars in the region of the Orion nebula.
o	Table 1, col(1): <PaCh NNN> (Nos 1-534). Table 1, col(4): <Haro 4-NNN> (Nos 256-495)
=E=	Catalogue in electronic form as <II/309/>
Details on Acronym: Haro
Haro	(Haro)= (HM) = (Haro 5-)
Write:	<<Haro 5-NN>>
N:	98
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Note:	Identif. charts.
in source:	IC 434
Ref:	=1953BOTT....1g..11H
by	HARO G. , MORENO A.
	Bol. Obs. Tonantz. Tacub., 1, part no 7, 11-22 (1953)
	Estrellas con Hα em emission en las cercanias de IC 434.
o	Table 1: <Haro 5-NN> (Nos 5-1 to 5-98).
Details on Acronym: Haro
Haro	(Haro)= (Haro 6-)
Write:	<<Haro 6-NN>>
N:	75
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Note:	2 Objects are PN: Haro 6-29 = PN H 3-29 = PN G174.2-14.6, Haro 6-75 = PN H 3-75 = PN G193.6-09.5.
Ref:	=1953BOTT....1h...3H
by	HARO G. , IRIARTE B., CHAVIRA E.
	Bol. Obs. Tonantz. Tacub., 1, part no 8, 3-18 (1953)
	Nuevas estrellas con emission en las regiones obscuras del Toro-Auriga-Orion investigadas por Joy.
o	Haro 6-29 = PN H 3-29, Haro 6-75 = PN H 3-75.
o	<Haro 6-NN> (Nos 6-1 to 6-75). <PN H 3-NN> N=2 (Nos 3-29, 3-75).
Details on Acronym: Haro
Haro	(Haro)= (Haro 7-)
Write:	<<Haro 7-NN>>
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Note:	p. 420: definition of the list Haro 7-: 'Unpublished. These objects were found marked on the original plates during a visit by Herbig to Tonantzintla in 1961. The numbers have been assigned arbitrarily'.
Ref:	=1972ApJ...174..401H
by	HERBIG G.H. , RAO N.K.
	Astrophys. J., 174, 401-423 (1972)
	Second catalog of emission-line stars of the Orion population.
o	Table 1: <HBC NNN> (Nos 1-323), <Em* LkHA NN> (Nos 321, 324-350). p. 420: <Haro 7-NN> unpublished.
Details on Acronym: Haro
Haro	(Haro)
*****	Avoid the usage of Haro, prefer [KH81]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Haro 1-
Haro 1-	(Haro)
*****	Avoid the usage of Haro 1-, prefer Haro
Details on Acronym: Haro 2-
Haro 2-	(Haro, list 2)
Note:	List Haro 2- is synonyme of PN H 1-NN (N=67)
*****	Avoid the usage of Haro 2-, prefer H
Details on Acronym: Haro 3-
Haro 3-	(Haro, list 3)
Note:	List Haro 3- is synonyme of PN H 2-NN (N=48)
*****	Avoid the usage of Haro 3-, prefer H
Details on Acronym: Haro 4-
Haro 4-	(Haro, list 4)
*****	Avoid the usage of Haro 4-, prefer Haro
Details on Acronym: Haro 5-
Haro 5-	(Haro, list 5)
*****	Avoid the usage of Haro 5-, prefer Haro
Details on Acronym: Haro 6-
Haro 6-	(Haro, list 6)
*****	Avoid the usage of Haro 6-, prefer Haro
Details on Acronym: Haro 7-
Haro 7-	(Haro, list 7)
*****	Avoid the usage of Haro 7-, prefer Haro
Details on Acronym: HaroChavira
HaroChavira	(Haro+Chavira)= (H-C)
Write:	<<HaroChavira NNN>>
N:	125
Object:	(IR) * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1965ApJ...142.1249J
by	JOHNSON H.L. , MENDOZA E.E., WISNIEWSKI W.Z.
	Astrophys. J., 142, 1249-1253 (1965)
	Observations of "infrared stars".
o	(Erratum) Vol. 144, p. 458
o	coordinates mis-precessed, see erratum for corrections.
o	Table 1: <HaroChavira N> (Nos 1-4, 6-8) (5 missing).
Ref:	=1967BOTT....4..197C
by	CHAVIRA E.
	Bol. Obs. Tonantz. Tacub., 4, 197-209 (1967)
	Lista preliminar de estrellas infrarrojas.
o	Tables 1, 2: <HaroChavira NNN> (Nos 9-126)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Harvard
Harvard	(Harvard univ.)
Write:	<<Cl Harvard NN>>
N:	47
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Details on Acronym: Harvard
Harvard	(Harvard univ., Variable *)
Write:	<<*SV HV** NNNNN>>
Object:	V* (SIMBAD class: Variable* = Variable Star)
Origin	of the Acronym: L (1924BAN.....2...82H)
Details on Acronym: [HAS2000]
[HAS2000]	(Handler+Arentoft+Shobbrook+, 2000)
Write:	<<[HAS2000] Star A>>
N:	2
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	N=2 stars in the field of XX Pyx.
Ref:	=2000MNRAS.318..511H
by	HANDLER G. , ARENTOFT T., SHOBBROOK R.R., WOOD M.A., CRAUSE L.A., CRAKE P., PODMORE F., HABANYAMA A., OSWALT T., BIRCH P.V., LOWE G., STERKEN C., MEINTJES P., BRINK J., CLAVER C.F., MEDUPE R., GUZIK J.A., BEACH T.E., MARTINEZ P., LEIBOWITZ E.M., IBBETSON P.A., SMITH T., ASHOKA B.N., RAJ N.E., KURTZ D.W., BALONA L.A., O'DONOGHUE D., COSTA J.E.S., BREGER M.
	Mon. Not. R. Astron. Soc., 318, 511-525 (2000)
	Delta Scuti Network observations of XX Pyx: detection of 22 pulsation modes and of short-term amplitude and frequency variations.
o	Fig.1: <[HAS2000] Star A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HAT
HAT	(Hungarian Automated Telescope network)
Write:	<<HAT FFF-NNNNNNN>>
N:	1617+383+120+1804
Object:	V* + * (SIMBAD class: Star)
Note:	Hungarian-made Automated Telescope network project. Only the first references are given here: 2004AJ....128.1761H: Search for variable stars in the field HAT 199. 2010MNRAS.408..475H: Search for variable stars in the Pleiades.
in source:	NAME Pleiades
Ref:	=2004AJ....128.1761H
by	HARTMAN J.D. , BAKOS G., STANEK K.Z., NOYES R.W.
	Astron. J., 128, 1761-1783 (2004)
	HATNET variability survey in the high stellar density ``Kepler field'' with millimagnitude image subtraction photometry.
o	Table 1: <HAT 199-NNNNN> N=1617 among about 98000.
Ref:	=2010MNRAS.408..475H
by	HARTMAN J.D. , BAKOS G.A., KOVACS G., NOYES R.W.
	Mon. Not. R. Astron. Soc., 408, 475-489 (2010)
	A large sample of photometric rotation periods for FGK Pleiades stars.
o	Tables 1-3: <HAT FFF-NNNNNNN> N=383+120+1804.
=E=	Catalogue in electronic form as J/AJ/128/1761
=E=	Catalogue in electronic form as <J/MNRAS/408/475/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HAT-P
HAT-P	(Hungarian Automated Telescope network, Planet)
Write:	<<HAT-P NN>> <<HAT-P NNa>>
Object:	* + Poss. Planet (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Detection of transiting planets (format NNa) within the HATNet projet. The associated stars have the format NN. The list of the discovered planets is available at: https://hatnet.org/planets/
Rem:	(a dash between the acronym and its contents is found in the literature)
Ref:	=2007ApJ...656..552B
by	BAKOS G.A. , NOYES R.W., KOVACS G., LATHAM D.W., SASSELOV D.D., TORRES G., FISCHER D.A., STEFANIK R.P., SATO B., JOHNSON J.A., PAL A., MARCY G.W., BUTLER R.P., ESQUERDO G.A., STANEK K.Z., LAZAR J., PAPP I., SARI P., SIPOCZ B.
	Astrophys. J., 656, 552-559 (2007)
	HAT-P-1b: a large-radius, low-density exoplanet transiting one member of a stellar binary.
o	<HAT-P N> (No. 1), <HAT-P Na> (No. 1b).
Ref:	=2007ApJ...665L.167W
by	WINN J.N. , JOHNSON J.A., PEEK K.M.G., MARCY G.W., BAKOS G.A., ENYA K., NARITA N., SUTO Y., TURNER E.L., VOGT S.S.
	Astrophys. J., 665L, 167-170 (2007)
	Spin-orbit alignment for the eccentric exoplanet HD 147506b.
o	<HAT-P N> (No. 2), <HAT-P Na> (No. 2b).
Ref:	=2007ApJ...666L.121T
by	TORRES G. , BAKOS G.A., KOVACS G., LATHAM D.W., FERNANDEZ J.M., NOYES R.W., ESQUERDO G.A., SOZZETTI A., FISCHER D.A., BUTLER R.P., MARCY G.W., STEFANIK R.P., SASSELOV D.D., LAZAR J., PAPP I., SARI P.
	Astrophys. J., 666L, 121-124 (2007)
	HAT-P-3b: a heavy-element-rich planet transiting a K dwarf star.
o	<HAT-P N> (No. 3), <HAT-P Na> (No. 3b).
Ref:	=2007ApJ...670L..41K
by	KOVACS G. , BAKOS G.A., TORRES G., SOZZETTI A., LATHAM D.W., NOYES R.W., BUTLER R.P., MARCY G.W., FISCHER D.A., FERNANDEZ J.M., ESQUERDO G., SASSELOV D.D., STEFANIK R.P., PAL A., LAZAR J., PAPP I., SARI P.
	Astrophys. J., 670L, 41-44 (2007)
	HAT-P-4b: a metal-rich low-density transiting hot Jupiter.
o	<HAT-P N> (No. 4), <HAT-P Na> (No. 4b).
Ref:	=2007ApJ...671L.173B
by	BAKOS G.A. , SHPORER A., PAL A., TORRES G., KOVACS G., LATHAM D.W., MAZEH T., OFIR A., NOYES R.W., SASSELOV D.D., BOUCHY F., PONT F., QUELOZ D., UDRY S., ESQUERDO G., SIPOCZ B., KOVACS G., STEFANIK R., LAZAR J., PAPP I., SARI P.
	Astrophys. J., 671L, 173-176 (2007)
	HAT-P-5b: a Jupiter-like hot Jupiter transiting a bright star.
o	<HAT-P N> (No. 5), <HAT-P Na> (No. 5b).
Ref:	=2008ApJ...673L..79N
by	NOYES R.W. , BAKOS G.A., TORRES G., PAL A., KOVACS G., LATHAM D.W., FERNANDEZ J.M., FISCHER D.A., BUTLER R.P., MARCY G.W., SIPOCZ B., ESQUERDO G.A., KOVACS G., SASSELOV D.D., SATO B., STEFANIK R., HOLMAN M., LAZAR J., PAPP I., SARI P.
	Astrophys. J., 673L, 79-82 (2008)
	HAT-P-6b: a hot Jupiter transiting a bright F star.
o	<HAT-P N> (No. 6), <HAT-P Na> (No. 6b).
Ref:	=2008ApJ...680.1450P
by	PAL A. , BAKOS G.A., TORRES G., NOYES R.W., LATHAM D.W., KOVACS G., MARCY G.W., FISCHER D.A., BUTLER R.P., SASSELOV D.D., SIPOCZ B., ESQUERDO G.A., KOVACS G., STEFANIK R., LAZAR J., PAPP I., SARI P.
	Astrophys. J., 680, 1450-1456 (2008)
	HAT-P-7b: an extremely hot massive planet transiting a bright star in the Kepler field.
o	<HAT-P N> (No. 7), <HAT-P Na> (No. 7b).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HATLAS
HATLAS	(Herschel ATLAS)
*****	Avoid the usage of HATLAS, prefer H-ATLAS
Origin	of the Acronym: L (2011MNRAS.416..680C)
Details on Acronym: HaTr
HaTr	(Hartl+Tritton)= (HtTr)
Write:	<<PN HaTr NN>>
N:	14
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Rem:	See ref. 1982AC D
Ref:	=1985A&A...145...41H
by	HARTL H. , TRITTON S.B.
	Astron. Astrophys., 145, 41-44 (1985)
	New planetary nebulae of low surface brightness detected on UK-Schmidt plates.
o	<PN HaTr NN> N=14
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HATS
HATS	(HATSouth survey)
Write:	<<HATS -NNA>> <<HATS -NNAa>>
Object:	* + Poss. Planet (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HATSouth network search for transiting exoplanets. Only the first references are listed here. The list of the discovered planets is available at: https://hatsouth.org/planets/
Rem:	(a dash between the acronym and its contents is found in the literature)
Ref:	=2013AJ....145....5P
by	PENEV K. , BAKOS G.A., BAYLISS D., JORDAN A., MOHLER M., ZHOU G., SUC V., RABUS M., HARTMAN J.D., MANCINI L., BEKY B., CSUBRY Z., BUCHHAVE L., HENNING T., NIKOLOV N., CSAK B., BRAHM R., ESPINOZA N., CONROY P., NOYES R.W., SASSELOV D.D., SCHMIDT B., WRIGHT D.J., TINNEY C.G., ADDISON B.C., LAZAR J., PAPP I., SARI P.
	Astron. J., 145, 5 (2013)
	HATS-1b: the first transiting planet discovered by the HATSouth survey.
o	<HATS-N> (No. 1). <HATS-Na> (No. 1b).
Ref:	=2013A&A...558A..55M
by	MOHLER-FISCHER M. , MANCINI L., HARTMAN J.D., BAKOS G.A., PENEV K., BAYLISS D., JORDAN A., CSUBRY Z., ZHOU G., RABUS M., NIKOLOV N., BRAHM R., ESPINOZA N., BUCHHAVE L.A., BEKY B., SUC V., CSAK B., HENNING T., WRIGHT D.J., TINNEY C.G., ADDISON B.C., SCHMIDT B., NOYES R.W., PAPP I., LAZAR J., SARI P., CONROY P.
	Astron. Astrophys., 558A, 55-55 (2013)
	HATS-2b: a transiting extrasolar planet orbiting a K-type star showing starspot activity.
Ref:	=2013AJ....146..113B
by	BAYLISS D. , ZHOU G., PENEV K., BAKOS G.A., HARTMAN J.D., JORDAN A., MANCINI L., MOHLER-FISCHER M., SUC V., RABUS M., BEKY B., CSUBRY Z., BUCHHAVE L., HENNING T., NIKOLOV N., CSAK B., BRAHM R., ESPINOZA N., NOYES R.W., SCHMIDT B., CONROY P., WRIGHT D.J., TINNEY C.G., ADDISON B.C., SACKETT P.D., SASSELOV D.D., LAZAR J., PAPP I., SARI P.
	Astron. J., 146, 113 (2013)
	HATS-3b: an inflated hot Jupiter transiting an f-type star.
=E=	Catalogue in electronic form as <J/A+A/558/A55/>
=E=	Catalogue in electronic form as <J/AJ/145/5/>
=E=	Catalogue in electronic form as <J/AJ/146/113/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HATS
HATS	(HATSouth survey)
*****	Avoid the usage of HATS, prefer [ZBH2014]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Haute-Provence
Haute-Provence	(Haute-Provence obs.)= (OHP) = (HP)
Write:	<<Cl Haute-Provence N>>
N:	5
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	No. 1 = An. (Dufay, Berthier, Morignat) = C 1727-299. Nos 2, 3, 4, 5 are Terzan 1, 2, 4, 6 respectively.
Details on Acronym: [HAV2011]
[HAV2011]	(Heiner+Allen+van der Kruit, 2011)
Write:	<<[HAV2011] Region 42>> <<[HAV2011] NN>> <<[HAV2011] NNa>>
N:	1+42+208
Object:	(FUV) + HI + Poss. PDR (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=42 prominent FUV sources in M33, each with multiple HI patches. Use of GALEX FUV and VLA 21-cm data.
in source:	M 33 = NGC 598
Ref:	=2011MNRAS.416....2H
by	HEINER J.S. , ALLEN R.J., VAN DER KRUIT P.C.
	Mon. Not. R. Astron. Soc., 416, 2-12 (2011)
	Atomic hydrogen produced in M33 photodissociation regions.
o	Table 3: <[HAV2011] Region 42> N=1. Table 5: <[HAV2011] NN> (Nos 1-42). Table 6: <[HAV2011] NNa> N=208.
=E=	Catalogue in electronic form as <J/MNRAS/416/2/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Havlen-Moffat
Havlen-Moffat	(Havlen+Moffat)
*****	Avoid the usage of Havlen-Moffat, prefer HM
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [HAW2008]
[HAW2008]	(Heiner+Allen+Wong+, 2008)
Write:	<<[HAW2008] NN>> <<[HAW2008] NNa>>
N:	76+638
Object:	Region + HI (SIMBAD class: PartofG = Part of a Galaxy)
Note:	GALEX Far-UV and VLA images of M 83. N=76 Photodissociation regions (PDR) and in these regions N=638 HI PEAK DENSITIES.
in source:	M 83 = NGC 5236
Ref:	=2008A&A...489..533H
by	HEINER J.S. , ALLEN R.J., WONG O.I., VAN DER KRUIT P.C.
	Astron. Astrophys., 489, 533-541 (2008)
	The volume densities of giant molecular clouds in M83.
o	Table 1: <[HAW2008] NN> (Nos 1-76). Table 3: <[HAW2008] NNa> N=638.
=E=	Catalogue in electronic form as J/A+A/489/533
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Hawaii
Hawaii	(Hawaii survey)
*****	Avoid the usage of Hawaii, prefer [CGH94]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Hawaii
Hawaii	(Hawaii survey)
*****	Avoid the usage of Hawaii, prefer [SCH94]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HAWC
HAWC	(High Altitude Water Cherenkov)
Write:	<<HAWC JHHMM+DDd>> <<HAWC -YYMMDDA>>
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	Tev gamma-ray sources (format JHHMM+DDd) and burst signals (format -YYMMDDA) reported by the High Altitude Water Cherenkov (HAWC) collaboration.
Ref:	=2017ATel10941....1R
by	RIVIERE C. , FLEISCHHACK H.
	The Astronomer's Telegram, 10941, 1 (2017)
	HAWC detection of TeV emission near PSR B0540+23.
Ref:	=2018ATel12013....1B
by	BRISBOIS C. , RIVIERE C., FLEISCHHACK H., SMITH A.
	ATel, 2013, 1 (2018)
	HAWC detection of TeV source HAWC J0635+070.
o	<HAWC JHHMM+DDd> (No. J0635+070).
Ref:	=2019GCN.26037....1H
by	HAWC COLLABORATION
	GCN, 6037, 1 (2019)
	Alert from the HAWC Burst Monitor HAWC-191019A.
o	<HAWC-YYMMDDA> (No. 191019A).
Ref:	=2020ApJ...896L..29A
by	ALBERT A. , ALFARO R., ALVAREZ C., ANGELES CAMACHO J.R., ARTEAGA-VELAZQUEZ J.C., ARUNBABU K.P., AVILA ROJAS D., AYALA SOLARES H.A., BAGHMANYAN V., BELMONT-MORENO E., BENZVI S.Y., BRISBOIS C., CABALLERO-MORA K.S., CAPISTRAN T., CARRAMINANA A., CASANOVA S., COTTI U., COTZOMI J., COUTINO DE LEON S., DE LA FUENTE E., DIAZ-CRUZ L., DINGUS B.L., DUVERNOIS M.A., DIAZ-VELEZ J.C., ELLSWORTH R.W., ENGEL K., ESPINOZA C., FAN K.L., FANG K., FERNANDEZ ALONSO M., FLEISCHHACK H., FRAIJA N., GALVAN-GAMEZ A., GARCIA D., GARCIA-GONZALEZ J.A., GARFIAS F., GIACINTI G., GONZALEZ M.M., GOODMAN J.A., HARDING J.P., HERNANDEZ S., HINTON J., HONA B., HUANG D., HUEYOTL-ZAHUANTITLA F., HUNTEMEYER P., IRIARTE A., JARDIN-BLICQ A., JOSHI V., LEE W.H., LEON VARGAS H., LINNEMANN J.T., LONGINOTTI A.L., LUIS-RAYA G., LUNDEEN J., MALONE K., MARINELLI S.S., MARTINEZ O., MARTINEZ-CASTELLANOS I., MARTINEZ-CASTRO J., MATTHEWS J.A., MIRANDA-ROMAGNOLI P., MORALES-SOTO J.A., MORENO E., MOSTAFA M., NAYERHODA A., NELLEN L., NEWBOLD M., NISA M.U., NORIEGA-PAPAQUI R., OMODEI N., PEISKER A., PEREZ ARAUJO Y., PEREZ-PEREZ E.G., RHO C.D., ROSA-GONZALEZ D., RUIZ-VELASCO E., SALAZAR H., SALESA GREUS F., SANDOVAL A., SCHNEIDER M., SCHOORLEMMER H., SERNA FRANCO J., SINNIS G., SMITH A.J., SPRINGER R.W., SURAJBALI P., TABACHNICK E., TANNER M., TIBOLLA O., TOLLEFSON K., TORRES I., TORRES-ESCOBEDO R., URENA-MENA F., VILLASENOR L., WEISGARBER T., ZEPEDA A., ZHOU H., DE LEON C., ALVAREZ J.D., (The HAWC Collaboration)
	Astrophys. J., 896L, 29-29 (2020)
	HAWC J2227+610 and its association with G106.3+2.7, a new potential Galactic PeVatron.
o	<HAWC JHHMM+DDd> (No. J2227+610).
Ref:	=2020GCN.28076....1H
by	HAWC COLLABORATION
	GCN, 8076, 1 (2020)
	Update of alert from the HAWC Burst Monitor HAWC-200709A.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HaWe
HaWe	(Hartl+Weinberger)= (HW)
Write:	<<PN HaWe NN>>
N:	15
Object:	Poss. PN (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
Stat:	is completely incorporated in Simbad
Note:	HaWe 3, 5, 9 are true PN in 1992, Acker+ catalog
Ref:	=1987A&AS...69..519H
by	HARTL H. , WEINBERGER R.
	Astron. Astrophys., Suppl. Ser., 69, 519-525 (1987)
	Planetary nebulae of low surface brightness : gleanings from the "POSS".
o	<PN HaWe NN> (Nos 1-15)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Hawk
Hawk	(Hawkins)= (SA287) = (Hawkins)
Write:	<<Hawk SA287 NNN>>
Object:	* (SIMBAD class: Star)
Note:	Hawkins, private communication, cited in 1995A&AS..109..171F
Auth.:	HAWKINS M.R.S.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HAWKI
HAWKI	(VLT HAWK-I) (Not yet in Simbad)
*****	Avoid the usage of HAWKI, prefer [GGV2016]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Hawkins
Hawkins	(Hawkins)
*****	Avoid the usage of Hawkins, prefer Hawk
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Hawkins
Hawkins	(Hawkins)
Write:	<<Hawkins NNN>> <<Hawkins RNN>> <<Hawkins VNN>>
N:	186+24+27
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Format 'NNN' for electronographic sequence of stars. Format 'RNN' for RR Lyrae stars (Nos R1-R26). Format 'VNN' for V*.
Ref:	=1981Natur.293..116H
by	HAWKINS M.R.S.
	Nature, 293, 116-120 (1981)
	Automated detection of variable objects on Scmidt plates.
o	<Hawkins VNN> N=27
Ref:	=1984MNRAS.206..433H
by	HAWKINS M.R.S.
	Mon. Not. R. Astron. Soc., 206, 433-448 (1984)
	A study of the galactic halo from a complete sample of RR Lyrae variables to B = 21.
o	Table 2: <Hawkins NNN> N=173 among (Nos 3-200), Table 4: <Hawkins RNN> (Nos R1-R26) R8 and R18 missing
Ref:	=1986MNRAS.223..845H
by	HAWKINS M.R.S.
	Mon. Not. R. Astron. Soc., 223, 845-858 (1986)
	On the nature of the missing mass in the solar neighbourhood.
o	Table 4: numbering 'MNN' is [HB88] MNN in SIMBAD.
o	Table 2, Plate 1: <Hawkins NNN> N=13 added among (Nos 201-218).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HB
HB	(Hakucho Burster) (Not yet in Simbad)
Write:	<<HB HHMM+DDd>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Details on Acronym: HB
HB	(Hawkins, sample B)
*****	Avoid the usage of HB, prefer [H86b]
Origin	of the Acronym: L (Veron)
Details on Acronym: HB
HB	(Hawkins+Bessell)
*****	Avoid the usage of HB, prefer [HB88]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HB
HB	(Hurt+Barsony)
*****	Avoid the usage of HB, prefer [HB96]
Origin	of the Acronym: L (1999AJ....118..558K)
Details on Acronym: HB
HB	(Hanbury Brown)
*****	Avoid the usage of HB, prefer HBH
Origin	of the Acronym: L (1999ARep...43..436P)
Details on Acronym: Hb
Hb	(Hubble)= (Hub) = (Hubble)
Write:	<<PN Hb NN>>
N:	9
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Hb 10, 11 are not PN
Ref:	=1921PASP...33..174H
by	HUBBLE E.P.
	Publ. Astron. Soc. Pac., 33, 174-175 (1921)
	Twelve new planetary nebulae.
o	Nos 10, 11 are not PN.
o	<PN Hb NN> N=10 among (Nos 1-12).
Details on Acronym: [HB2004]
[HB2004]	(Humphrey+Buote, 2004)
Write:	<<[HB2004] NN>>
N:	73
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-S3 observations of the galaxy NGC 1332.
in source:	NGC 1332
Ref:	=2004ApJ...612..848H
by	HUMPHREY P.J. , BUOTE D.A.
	Astrophys. J., 612, 848-859 (2004)
	A Chandra view of the normal S0 galaxy NGC 1332. I. An unbroken, steep power-law luminosity function for the low-mass X-ray binary population.
o	Table 1: <[HB2004] NN> (Nos 1-73).
=E=	Catalogue in electronic form as J/ApJ/612/848
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HB2006]
[HB2006]	(Hui+Becker, 2006)
Write:	<<[HB2006] A>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra HRC observations of RX J0822.0-4300 in the SNR Pup A.
in source:	NAME Puppis A
Ref:	=2006A&A...457L..33H
by	HUI C.Y. , BECKER W.
	Astron. Astrophys., 457L, 33-36 (2006)
	Probing the proper motion of the central compact object in Puppis-A with the Chandra high resolution camera.
o	Table 1: <[HB2006] A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HB2008]
[HB2008]	(Hanson+Bubnick, 2008)
Write:	<<[HB2008] CL 107 NNN>> <<[HB2008] CL 107 No. NNN>> (not recognised by Simbad, but found in literature)
N:	130
Object:	* in Cl* (SIMBAD class: Star)
Note:	IRTF spectroscopy of the cluster [BDS2003] 107.
in source:	[BDS2003] 107
Ref:	=2008PASP..120..150H
by	HANSON M.M. , BUBNICK B.F.
	PASP, 120, 150-159 (2008)
	Near-infrared spectroscopy of candidate members of the galactic cluster [BDS2003] 107.
o	Table 1: <[HB2008] CL 107 NNN> (Nos 1-130).
=E=	Catalogue in electronic form as J/PASP/120/150
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HB2009]
[HB2009]	(Hui+Becker, 2009)
Write:	<<[HB2009] NN>>
N:	36
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-I observations of the field of SNR 67.7+1.8.
Ref:	=2009A&A...494.1005H
by	HUI C.Y. , BECKER W.
	Astron. Astrophys., 494, 1005-1012 (2009)
	Exploring the X-ray emission properties of the supernova remnant G67.7+1.8 and its central X-ray sources.
o	Table 1: <[HB2009] NN> (Nos 1-36).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HB2010]
[HB2010]	(Hutchings+Bianchi, 2010)= ([HB2010a])
Write:	<<[HB2010] NN>>
N:	10
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=10 bright galaxies in a GALEX-SDSS sample. Use of SDSS spectroscopy.
Ref:	=2010AJ....139..630H
by	HUTCHINGS J.B. , BIANCHI L.
	Astron. J., 139, 630-635 (2010)
	Luminous star-forming galaxies in the galaxy evolution Explorer-Sloan Digital Sky Survey database.
o	Table 1: <[HB2010] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HB2010a]
[HB2010a]	(Hutchings+Bianchi, 2010)
*****	Avoid the usage of [HB2010a], prefer [HB2010]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HB2010b]
[HB2010b]	(Heithausen+Boettner, 2010)
Write:	<<[HB2010b] L 1457-AN>> <<[HB2010b] J025616+192703>>
N:	4+1
Object:	mm Condensation + (Rad) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	IRAM 30m MAMBO 1.2mm and VLA 3.6cm observations of dust condensations in LDN 1457.
in source:	LDN 1457
in source:	MBM 12
Ref:	=2010A&A...521L..58H
by	HEITHAUSEN A. , BOETTNER C.
	Astron. Astrophys., 521L, 58-58 (2010)
	A candidate protostellar object in the L 1457/MBM 12 cloud.
o	Fig. 1, Table 1: <[HB2010b] L 1457-AN> (Nos A-C, C1). Table 3: <[HB2010b] J025616+192703> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HB88]
[HB88]	(Hawkins+Bessell, 1988)= (HB)
Write:	<<[HB88] NN>> <<[HB88] {S\|M\|N}NN>> <<[HB88] HHMM+DDMM>>
N:	37
Object:	* (SIMBAD class: Star)
Note:	Table 3: N=14 * at SGP, among (Nos 5-36). Table 5: in the format, the letters S or M or N stands for spectral type. N=5 among (Nos S1-S6). N=8 among (Nos M1-M20), N=11 already studied in 1986MNRAS.223..845H. N=4 among (Nos N1-N7).
Ref:	=1988MNRAS.234..177H
by	HAWKINS M.R.S. , BESSELL M.S.
	Mon. Not. R. Astron. Soc., 234, 177-191 (1988)
	The luminosity function for low mass stars.
o	Table 3: <[HB88] NN> N=14 among (Nos 5-36), Table 5: <[HB88] ANN> N=5 among (Nos S1-S6), N=8 among (Nos M1-M20), N=4 among (Nos N1-N7)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HB89]
[HB89]	(Hewitt+Burbidge, 1989)
Note:	Superseded by [HB93]
*****	Avoid the usage of [HB89], prefer [HB93]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HB91]
[HB91]	(Hewitt+Burbidge, 1991)= ([HB91a])
Write:	<<[HB91] HHMM+DDdA>>
N:	935
Object:	AGN (SIMBAD class: AGN = Active Galaxy Nucleus)
Note:	The authors used a format 'HHMM+DDd', but there are ambigus cases such as 2359-899 so we have to use the format 'HHMM+DDdA', 2359-899A to 2359-899D for example. Superseded by [HB93]
Ref:	=1991ApJS...75..297H
by	HEWITT A. , BURBIDGE G.
	Astrophys. J., Suppl. Ser., 75, 297-356 (1991)
	An optical catalog of extragalactic emission-line objects similar to quasi-stellar objects.
o	Catalogue: <[HB91] HHMM+DDdA> N=935.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HB91a]
[HB91a]	(Hewitt+Burbidge, 1991)
*****	Avoid the usage of [HB91a], prefer [HB91]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HB91b]
[HB91b]	(Henry+Briel, 1991)
Write:	<<[HB91b] NN>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT observations of ACO 2256.
in source:	ACO 2256
Ref:	=1991A&A...246L..14H
by	HENRY J.P. , BRIEL U.G.
	Astron. Astrophys., 246, 14-16 (1991)
	The X-ray morphology of the relaxed cluster of galaxies A 2256. II. Sources around the extended cluster emission.
o	Table 1: <[HB91b] NN> (Nos 1-23).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HB93]
[HB93]	(Hewitt+Burbidge, 1993)= (BL) = [HB89]
Write:	<<[HB93] HHMM+DDdA>>
N:	7315
Object:	QSO (SIMBAD class: QSO = Quasar)
Note:	The authors used a format 'HHMM+DDd', but there are ambiguous cases such as 0002-008 so we have to use the format 'HHMM+DDdA', 0002-008A and 0002-008B for example. Supersedes [HB91]
Ref:	=1993ApJS...87..451H
by	HEWITT A. , BURBIDGE G.
	Astrophys. J., Suppl. Ser., 87, 451-None (1993)
	A revised and updated catalog of quasi-stellar objects.
o	Table 1: <[HB93] HHMM+DDdA> N=7315
=E=	Catalogue in electronic form as VII/158
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HB94]
[HB94]	(Heydari-Malayeri+Beuzit, 1994)
Write:	<<[HB94] Sk -66 41 NN>>
N:	12
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Come-on-Plus observations on ESO 3.6m telescope. N=12 stars in 'Sk -66 41 cluster'. See also [HMR88], [HRR2000].
in source:	NAME SK -66 41 Cluster
Ref:	=1994A&A...287L..17H
by	HEYDARI-MALAYERI M. , BEUZIT J.-L.
	Astron. Astrophys., 287, 17-20 (1994)
	Further decomposition of a "very massive" star.
o	Table 1: <[HB94] Sk -66 41 NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HB96]
[HB96]	(Hurt+Barsony, 1996)= (HB) = (PS)
Write:	<<[HB96] PS N>>
N:	2
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	IRAS images. In the format 'PS N' (Nos 1-2), the letters 'PS' stand for Point Source.
Ref:	=1996ApJ...460L..45H
by	HURT R.L. , BARSONY M.
	Astrophys. J., 460, 45-48 (1996)
	A cluster of class 0 protostars in Serpens: an IRAS HIRES study.
o	<[HB96] PS N> (Nos 1-2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HB98]
[HB98]	(Hughes+Birkinshaw, 1998)
Write:	<<[HB98] N>> <<[HB98] a>>
N:	8+7
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table 1: (Nos 1-8) are G in ClG 0016+16, (Nos a-g) are G probable non members.
in source:	ClG 0016+1609 = 1E 0015.9+1609
Ref:	=1998ApJ...497..645H
by	HUGHES J.P. , BIRKINSHAW M.
	Astrophys. J., 497, 645-649 (1998)
	Another X-ray-discovered poor cluster of galaxies associated with CL 0016+16.
o	Table 1: <[HB98] N> (Nos 1-8), <[HB98] a> (Nos a-g).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBA99]
[HBA99]	(Hurst+Boles+Armstrong+, 1999)
Write:	<<[HBA99] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=1 host galaxy of SN 1999BT
Ref:	=1999IAUC.7142Q...1H
by	HURST G.M. , BOLES T., ARMSTRONG M., JHA S., GARNAVICH P., CHALLIS P., KIRSHNER R., CALKINS M., MACRI L.
	IAU Circ., 7142, 1-None (1999)
	Supernova 1999bt in anonymous galaxy.
o	<[HBA99] JHHMMSS.ss-DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBB99]
[HBB99]	(Huang+Bania+Bolatto+, 1999)
Write:	<<[HBB99] LLL.lll+B.bbb>>
N:	49
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	AST/RO observations. N=49 southern hemisphere HII regions. Objects from [WMG70], with an extended format. See also [WMG70].
Ref:	=1999ApJ...517..282H
by	HUANG M. , BANIA T.M., BOLATTO A., CHAMBERLIN R.A., INGALLS J.G., JACKSON J.M., LANE A.P., STARK A.A., WILSON R.W., WRIGHT G.A.
	Astrophys. J., 517, 282-291 (1999)
	Atomic carbon observations of southern hemisphere H II regions.
o	Table 1: <[HBB99] LLL.lll+B.bbb> N=49.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HBC
HBC	(Herbig+Bell, Catalog)= (HRC)
Write:	<<HBC NNN>>
N:	742
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-742) this catalog replaces the second catalog (HRC, ref. 1972ApJ...174..401H) and adds (Nos 324-742). the HRC acronym is superseded by HBC. The letter 'n' or an asterisk are not part of the designation, but are separate items of information: n means star embedded in a nebulosity. ref. 1992ApJS...78..239W cross-id. HBC with IRAS PSC catalog
Ref:	=1988LicOB1111....1H
by	HERBIG G.H. , BELL K.R.
	Lick Obs. Bull., 1111, 1-90 (1988)
	Third catalog of emission-line stars of the Orion population.
o	in ref list GLEDHILL 1986MNRAS.223..867G instead of 230.867, HERBIG 196 3ApJ...137..398H instead of 1953
o	<HBC NNN> (Nos 1-742)
=E=	Catalogue in electronic form as V/73
=E=	Catalogue in electronic form as <V/73A/>
Details on Acronym: [HBC2005]
[HBC2005]	(Honma+Bushimata+Choi+, 2005) (Not yet in Simbad)
Write:	<<[HBC2005] NN>>
N:	43
Object:	H2O Maser (SIMBAD class: Maser)
Note:	Search for H2O maser emission in OH 43.8-0.1.
in source:	OH 43.8 -0.1
Ref:	=2005PASJ...57..595H
by	HONMA M. , BUSHIMATA T., CHOI Y.K., FUJII T., HIROTA T., HORIAI K., IMAI H., INOMATA N., ISHITSUKA J., IWADATE K., JIKE T., KAMEYA O., KAMOHARA R., KAN-YA Y., KAWAGUCHI N., KIJIMA M., KOBAYASHI H., KUJI S., KURAYAMA T., MANABE S., MIYAJI T., NAKAGAWA A., NAKASHIMA K., OH C.S., OMODAKA T., OYAMA T., RIOJA M., SAKAI S., SATO K., SASAO T., SHIBATA K., SHIMIZU R., SORA K., SUDA H., TAMURA Y., YAMASHITA K.
	Publ. Astron. Soc. Jap., 57, 595-603 (2005)
	Multi-epoch VERA observations of H_{2}O masers in OH 43.8-0.1.
o	Table 1: <[HBC2005] NN> (Nos 1-43).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBC2014]
[HBC2014]	(Hunter+Brogan+Cyganowsk+, 2014)
Write:	<<[HBC2014] VLA N>> <<[HBC2014] H2O-C4>>
N:	2
Object:	(cm) (SIMBAD class: cmRad = Centimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 6cm observations of N=2 radio sources in the field of the NGC 6334 I(N) protocluster.
in source:	NGC 6334:MFSW I(N) = MFSW I(N)
Ref:	=2014ApJ...788..187H
by	HUNTER T.R. , BROGAN C.L., CYGANOWSKI C.J., YOUNG K.H.
	Astrophys. J., 788, 187 (2014)
	Subarcsecond imaging of the NGC 6334 I(N) protocluster: two dozen compact sources and a massive disk candidate.
o	Table 2: <[HBM2006b] I(N)-SMANNa> N=16 (Nos I(N)-SMA8 to I(N)-SMA23) added. Table 3: <[HBC2014] VLA N> (No VLA 2), <[HBC2014] H2O-C4> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBC92]
[HBC92]	(Huggins+Bachiller+Cox+, 1992)
Write:	<<[HBC92] AN>> <<[HBC92] HHMMSS.s+DDMMSS>>
N:	5+1
Object:	Globule + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=5 CO condensations in 3 fields A to C, in Helix nebula. These condensations are localized at the positions of globules. Central star is [HBC92] 222654.7-210537.
in source:	Helix Nebula = NGC 7293
Ref:	=1992ApJ...401L..43H
by	HUGGINS P.J. , BACHILLER R., COX P., FORVEILLE T.
	Astrophys. J., 401, 43-46 (1992)
	CO in the cometary globules of the Helix Nebula.
o	Paragr.2: 1950 coordinates of the central star: Dec at -20° is a misprint for -21 °.
o	Table 1: <[HBC92] AN> (Nos A1-A2, B1, C1-C2). Text: <[HBC92] HHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBC93]
[HBC93]	(Hill+Bohlin+Cheng+, 1993)= (H93)
Write:	<<[HBC93] NNN>>
N:	314
Object:	* (SIMBAD class: Star)
Note:	UIT observations aboard Astro-1. Photometry of stars in 30 Dor nebula.
in source:	Magellanic Clouds:LMC:30 Dor Nebula = 30 Dor Nebula
Ref:	=1993ApJ...413..604H
by	HILL J.K. , BOHLIN R.C., CHENG K.-P., FANELLI M.N., HINTZEN P., O'CONNELL R.W., ROBERTS M.S., SMITH A.M., SMITH E.P., STECHER T.P.
	Astrophys. J., 413, 604-610 (1993)
	30 Doradus : ultraviolet and optical stellar photometry.
o	Table 3: <[HBC93] NNN> (Nos 0-313).
=E=	Catalogue in electronic form as J/ApJ/413/604
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBC96]
[HBC96]	(Henry+Balkowski+Cayatte+, 1996)
Write:	<<[HBC96] NN>>
N:	26
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Finding chart in Fig. 1
in source:	NGC 753
Ref:	=1996MNRAS.283..635H
by	HENRY R.B.C. , BALKOWSKI C., CAYATTE V., EDMUNDS M.G., PAGEL B.E.J.
	Mon. Not. R. Astron. Soc., 283, 635-647 (1996)
	The effects of cluster environment on the chemical evolution of galaxies. III. NGC 753.
o	Table 1: <[HBC96] NN> (Nos 1-26)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBC97]
[HBC97]	(Hamann+Beaver+Cohen+, 1997)
Write:	<<[HBC97] A>> <<[HBC97] NN>>
N:	1+19
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of PKS 2135-147. Table 1: Sources in the PKS field: No. A (ref. 1982ApJ...257...33S) and (Nos 1-19). (Nos 1-3) are identical to [S78e] 2135-147 N (Nos 1-3)
Ref:	=1997ApJ...488..155H
by	HAMANN F. , BEAVER E.A., COHEN R.D., JUNKKARINEN V., LYONS R.W., BURBIDGE E.M.
	Astrophys. J., 488, 155-163 (1997)
	The nature and origin of z_{a} ≃ z_{e} absorption lines in the redshift 0.20 quasar PKS 2135-147.
o	Table 1: <[HBC97] A> N=1, No. A, <[HBC97] NN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBD2007]
[HBD2007]	(Haberzettl+Bomans+Dettmar+, 2007)= (LSB)
Write:	<<[HBD2007] LSB JHHMMm+DDMMm>>
N:	37
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Search for LSB galaxies in the HDFS.
in source:	NAME HDFS
Ref:	=2007A&A...465...95H
by	HABERZETTL L. , BOMANS D.J., DETTMAR R.-J., POHLEN M.
	Astron. Astrophys., 465, 95-105 (2007)
	Low surface brightness galaxies around the HDF-S. I. Object extraction and photometric results.
o	Table 3: <[HBD2007] LSB JHHMMm+DDMMm> N=37.
=E=	Catalogue in electronic form as J/A+A/465/95
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBD2009]
[HBD2009]	(Hales+Barlow+Drew+, 2009)
Write:	<<[HBD2009] WHT JHHMMSS+DDMMSS>> <<[HBD2009] IPHAS JHHMMSS+DDMMSS>>
N:	10+17
Object:	* (SIMBAD class: Star)
Note:	IPHAS A-stars in the Galactic Plane cross-correlated with Spitzer data. WHT spectroscopy of N=10 stars.
Ref:	=2009ApJ...695...75H
by	HALES A.S. , BARLOW M.J., DREW J.E., UNRUH Y.C., GREIMEL R., IRWIN M.J., GONZALEZ-SOLARES E.
	Astrophys. J., 695, 75-93 (2009)
	IPHAS A-type stars with mid-infrared excesses in Spitzer surveys.
o	Table 4: <[HBD2009] WHT JHHMMSS+DDMMSS> N=10. Tables 6-7: <[HBD2009] IPHAS JHHMMSS+DDMMSS> N=17.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HbDs
HbDs	(Heber+Drilling)
Write:	<<PN HbDs N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	HbDs 1 = PN G049.3+88.1 = PK 049+88 1
Ref:	=1984MitAG..62..252H
by	HEBER U. , DRILLING J.S.
	Mitt. Astron. Gesellschaft, 62, 252-None (1984)
	High resolution spectroscopy of the CPN LSS 1362.
o	<PN HbDs 1>
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HBE2010]
[HBE2010]	(Huang+Becker+Edmonds+, 2010)
Write:	<<[HBE2010] sNNa>>
N:	38
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST WFPC2 observations of the globular cluster M 71. See also [EHC2008].
in source:	M 71 = NGC 6838
Ref:	=2010A&A...513A..16H
by	HUANG R.H.H. , BECKER W., EDMONDS P.D., ELSNER R.F., HEINKE C.O., HSIEH B.C.
	Astron. Astrophys., 513A, 16-16 (2010)
	Study of Hubble space telescope counterparts to Chandra X-ray sources in the globular cluster M71.
o	Table 2: <[HBE2010] sNNa> N=38 among (Nos s01-s54b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Hbg
Hbg	(Heidelberg objective prism survey)= (KS)
Write:	<<Hbg NNNN>>
N:	1660
Object:	OB* (SIMBAD class: Star)
Note:	MK spectral types for 1113 stars are given in ref. 1977ApJS...35..111G
Ref:	=1966VeHei..18....9K
by	KLARE G. , SZEIDL B.
	Veroeff. des Badischen Sternw. Heidelberg, 18, 9-50 (1966)
	OB stars in the Southern Milky Way.
o	<Hbg NNNN> (Nos 1-1660).
Details on Acronym: [HBG2001]
[HBG2001]	(Hornschemeier+Brandt+Garmire+, 2001)= (HDFX)
Write:	<<[HBG2001] NN>>
N:	82
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of the HDFN. See also CXOHDFN.
in source:	NAME HDF
Ref:	=2001ApJ...554..742H
by	HORNSCHEMEIER A.E. , BRANDT W.N., GARMIRE G.P., SCHNEIDER D.P., BARGER A.J., BROOS P.S., COWIE L.L., TOWNSLEY L.K., BAUTZ M.W., BURROWS D.N., CHARTAS G., FEIGELSON E.D., GRIFFITHS R.E., LUMB D., NOUSEK J.A., RAMSEY L.W., SARGENT W.L.W.
	Astrophys. J., 554, 742-777 (2001)
	The Chandra deep survey of the Hubble Deep Field-north area. II. Results from the Caltech faint field galaxy redshift survey area.
o	Table 4, col(1): <[HBG2001] NN> (Nos 1-82) = <CXOHDFN JHHMMSS.s+DDMMSS> N=82.
=E=	Catalogue in electronic form as J/ApJ/554/742
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBG2012]
[HBG2012]	(Hall+Bradac+Gonzalez+, 2012)
Write:	<<[HBG2012] NN>> <<[HBG2012] A>>
N:	10+12
Object:	High redshift G + G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFC3 observations of N=10 z850-dropout galaxies and N=12 z850- and J110-dropout contaminants in the Bullet Cluster field.
in source:	NAME Bullet Cluster
Ref:	=2012ApJ...745..155H
by	HALL N. , BRADAC M., GONZALEZ A.H., TREU T., CLOWE D., JONES C., STIAVELLI M., ZARITSKY D., CUBY J.-G., CLEMENT B.
	Astrophys. J., 745, 155 (2012)
	Using the bullet cluster as a gravitational telescope to study z ≳ 7 Lyman break galaxies.
o	Fig. 3, Table 1: <[HBG2012] NN> (Nos 1-10). Fig. 4, Table 2: <[HBG2012] A> (Nos A-L).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBG2016]
[HBG2016]	(Hamren+Beaton+Guhathakurta+, 2016)
Write:	<<[HBG2016] NNNNNNNN>> <<[HBG2016] osN>>
N:	41
Object:	C* (SIMBAD class: C* = Carbon Star)
Note:	Keck DEIMOS observations of N=41 carbon stars in the satellites and halo of M31 as part of the SPLASH survey.
in source:	M 31
Ref:	=2016ApJ...828...15H
by	HAMREN K. , BEATON R.L., GUHATHAKURTA P., GILBERT K.M., TOLLERUD E.J., BOYER M.L., ROCKOSI C.M., SMITH G.H., MAJEWSKI S.R., HOWLEY K.
	Astrophys. J., 828, 15-15 (2016)
	Carbon stars in the satellites and halo of M31.
o	Table 2: <[HBG2016] NNNNNNNN> N=40 (Nos 131-60001744), Table 2: <[HBG2016] osN> N=1 (No os2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBG98]
[HBG98]	(Hasinger+Burg+Giacconi+, 1998)
*****	Avoid the usage of [HBG98], prefer RDS
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HBH
HBH	(Hanbury Brown+Hazard)= (HB)
Write:	<<HBH NN>>
N:	23
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Ref:	=1953MNRAS.113..123H
by	HANBURY BROWN R. , HAZARD C.
	Mon. Not. R. Astron. Soc., 113, 123-133 (1953)
	A survey of 23 localized radio sources in the Northern hemisphere.
o	Table I: <HBH NN> (Nos 1-23)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HBH
HBH	(Hamburg-Bergedorf, H-alpha)
*****	Avoid the usage of HBH, prefer HBHA
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HBH2013]
[HBH2013]	(Heywood+Bielby+Hill+, 2013)
Write:	<<[HBH2013] WHDF-EVLA-NN>> <<[HBH2013] JHHMMSS.ss+DDMMSS.s>>
N:	41+22
Object:	(Rad) + (Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Expanded VLA (EVLA) observations at 8.4GHz of N=41 radio sources in the William Herschel Deep Field. Use of existing optical observations of N=22 possible optical counterpartsi (including Magellan-1 6.5m telescope LDSS2 spectroscopy of eight of those sources).
in source:	NAME Herschel Deep Field
Ref:	=2013MNRAS.428..935H
by	HEYWOOD I. , BIELBY R.M., HILL M.D., METCALFE N., RAWLINGS S., SHANKS T., SMIRNOV O.M.
	Mon. Not. R. Astron. Soc., 428, 935-951 (2013)
	Sub-millimetre source identifications and the microjansky source population at 8.4GHz in the William Herschel Deep Field.
o	Table 1: <[HBH2013] WHDF-EVLA-NN> (Nos 1-41). Table 2: <[HBH2013] JHHMMSS.ss+DDMMSS.s> N=22.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBH2015]
[HBH2015]	(Hoag+Bradac+Huang+, 2015)= ([HBH2015a])
Write:	<<[HBH2015] RCS2327-NNNN>>
N:	5
Object:	High redshift G (SIMBAD class: Galaxy)
Note:	HST ACS and WFC3 photometry and Keck MOSFIRE spectroscopy of the galaxy cluster RCS J2327-0204, as part of the Spitzer Ultra Faint Survey Program (SURFSUP). N=5 F814W-dropout candidates (N=4 primary dropout and N=1 secondary dropout) at z∼7 were detected.
in source:	RCS J2327-0204
Ref:	=2015ApJ...813...37H
by	HOAG A. , BRADAC M., HUANG K.H., RYAN R.E.Jr, SHARON K., SCHRABBACK T., SCHMIDT K.B., CAIN B., GONZALEZ A.H., HILDEBRANDT H., HINZ J., LEMAUX B.C., VON DER LINDEN A., LUBIN L.M., TREU T., ZARITSKY D.
	Astrophys. J., 813, 37 (2015)
	RCS2 J232727.6-020437: an efficient cosmic telescope at z=0.6986.
o	Table 3, Fig. 1: <[SGM2015] RCS2327 A> (Nos C-G) added, <[SGM2015] RCS2327 A.N> N=10 added, <[SGM2015] RCS2327 A.Nc> N=6 added. Table 4, Text: <[HBH2015] RCS2327-NNNN≥5 among (Nos 843-2068).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBH2015a]
[HBH2015a]	(Hoag+Bradac+Huang+, 2015)
*****	Avoid the usage of [HBH2015a], prefer [HBH2015]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBH2015b]
[HBH2015b]	(Huynh+Bell+Hopkins+, 2015) (Not yet in Simbad)
Write:	<<[HBH2015b] NNN>> <<[HBH2015b] NNNA>>
N:	189+12
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ATCA 5.5GHz observations of N=189 sources (format NNN) and N=12 multiple component sources (format NNNA) in the extended Chandra Deep Field South, by the Australia Telescope Large Area Survey (ATLAS) team. See also ATCDFS5, [HHL2012], as well as ATCDFS9, [HSN2020].
in source:	NAME ECDFS
Ref:	=2015MNRAS.454..952H
by	HUYNH M.T. , BELL M.E., HOPKINS A.M., NORRIS R.P., SEYMOUR N.
	Mon. Not. R. Astron. Soc., 454, 952-972 (2015)
	The ATLAS 5.5 GHz survey of the extended Chandra Deep Field-South: the second data release.
o	Table 2, col(1): <[HBH2015b] NNN> (Nos 1-189), <[HBH2015b] NNN> N=12 among (Nos 20A-20B to 177A-177B). Table 2, col(2): <ATCDFS5 JHHMMSS.ss+DDMMSS.s> N=212.
=E=	Catalogue in electronic form as <J/MNRAS/454/952/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBH2019]
[HBH2019]	(Hoag+Bradac+Huang+, 2019)
Write:	<<[HBH2019] ANNNN-NNN>> <<[HBH2019] MACSHHMM-NNN>> <<[HBH2019] RXJ1347-NNN>> <<[HBH2019] RCS2327-NNN>>
N:	70
Object:	Poss. LBG (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck I MOSFIRE spectroscopy of N=70 Lyman-break galaxies (LBGs) behind 12 galaxy cluster lenses.
Ref:	=2019ApJ...878...12H
by	HOAG A. , BRADAC M., HUANG K., MASON C., TREU T., SCHMIDT K.B., TRENTI M., STRAIT V., LEMAUX B.C., FINNEY E.Q., PADDOCK M.
	Astrophys. J., 878, 12-12 (2019)
	Constraining the neutral fraction of hydrogen in the IGM at redshift 7.5.
o	Table 5: <[HBH2019] ANNNN-NNN>, <[HBH2019] MACSHHMM-NNN>, <[HBH2019] RXJ1347-NNN>, <[HBH2019] RCS2327-NNN>, N=70.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBH95]
[HBH95]	(Hunter+Boyd+Hawley, 1995)
Write:	<<[HBH95] M33-NNN NNNN>> <<[HBH95] M33-ZNNN NNNN>> <<[HBH95] M31-B2 NNNN>>
N:	2090+138
Object:	* (SIMBAD class: Star)
Note:	Table 2: N=2090 * in M 33. in the format 'M33-NNN' and 'M33-ZNNN' stands for 5 regions each region is divided into 5 groups (Nos 1-5) corresponding to the 1st digit in the numbering 'NNNN' (always a 4 digits format) stars in each group are numbered 'NNN' (3 last digits). Table 2: N=138 * in M 31. in the region 'M31-B2' and the same numbering 'NNNN' as in M 33
in source:	M 31 = NGC 224
in source:	M 33 = NGC 598
Ref:	=1995ApJS...99..551H
by	HUNTER D.A. , BOYD D.M., HAWLEY W.N.
	Astrophys. J., Suppl. Ser., 99, 551-563 (1995)
	The massive star populations in ionized gas shells in M33 and M31.
o	Table 2: <[HBH95] M33-NNN NNNN>, <[HBH95] M33-ZNNN NNNN> N=2090, <[HBH95] M31-B2 NNNN> N=138
=E=	Catalogue in electronic form as J/ApJS/99/551
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HBHA
HBHA	(Hamburg-Bergedorf, H-Alpha)= (HBH)
Write:	<<HBHA NNNN-NN>> <<HBHA -NNNN-NN>>
N:	1984
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Note:	Catalogue of H-alpha emission stars: see [KW97]. The HBH list (main list, Schmidt camera Hamburg-Bergedorf, red plates taken in the years 1964-70) contains 1984 objects partly identical with those in other lists of H emission-line stars given in the literature up till 1994.
Ref:	=1997AAHam..11....1K
by	KOHOUTEK L. , WEHMEYER R.
	Astron. Abh. Hamburg. Sternw., 11, 1-None (1997)
	Catalogue of stars in the Northern Milky Way having H-α in emission.
o	Catalog, Col(1): <[KW97] pp-NN> N=4174. Catalog, Col(19): <HBHA NNNN-NN> N=1984.
Ref:	=1999A&AS..134..255K
by	KOHOUTEK L. , WEHMEYER R.
	Astron. Astrophys., Suppl. Ser., 134, 255-256 (1999)
	Catalogue of H-α emission stars in the Northern Milky Way.
o	The catalogue was first reported in 1997AAHam..11....1K
o	Catalog, Col(1): <[KW97] pp-NN> N=4174. Catalog, Col(19): <HBHA NNNN-NN> N=1984.
=E=	Catalogue in electronic form as III/205
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBI2008]
[HBI2008]	(Hunter+Brogan+Indebetouw+, 2008)
Write:	<<[HBI2008] SMAN>> <<[HBI2008] SMA-W>>
N:	2+3
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SubMillimeter Array (SMA) 875mu.m observations of the HII region Gal 5.89-0.39.
in source:	GAL 005.89-00.39
Ref:	=2008ApJ...680.1271H
by	HUNTER T.R. , BROGAN C.L., INDEBETOUW R., CYGANOWSKI C.J.
	Astrophys. J., 680, 1271-1288 (2008)
	Subarcsecond submillimeter imaging of the ultracompact H II region G5.89-0.39.
o	Fig.1, Table 4: <[HBI2008] SMAN> (Nos SMA1, SMA2), <[HBI2008] SMA-W> (Nos N, S, E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBJ2002]
[HBJ2002]	(Hjorth+Burud+Jaunsen+, 2002)
Write:	<<[HBJ2002] RN>>
N:	3
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=3 reference stars in the field of RX J0911.4+0551.
Ref:	=2002ApJ...572L..11H
by	HJORTH J. , BURUD I., JAUNSEN A.O., SCHECHTER P.L., KNEIB J.-P., ANDERSEN M.I., KORHONEN H., CLASEN J.W., KAAS A.A., OSTENSEN R., PELT J., PIJPERS F.P.
	Astrophys. J., 572, 11-14 (2002)
	The time delay of the quadruple quasar RX J0911.4+0551.
o	Fig.2: stars S1, S2 not identified.
o	Table 1: <[HBJ2002] RN> (Nos R1-R3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBJ2010]
[HBJ2010]	(Hickey+Bunker+Jarvis+, 2010)
Write:	<<[HBJ2010] NNNN>> <<[HBJ2010] JHHMMSS.s+DDMMSS.s>>
N:	8+2
Object:	G + Transient (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT Hawk-I NIR observations of galaxies in the GOODS-South field. Use of HST ACS, VLT ISAAC and Spitzer IRAC data.
in source:	NAME GOODS South Field
Ref:	=2010MNRAS.404..212H
by	HICKEY S. , BUNKER A., JARVIS M.J., CHIU K., BONFIELD D.
	Mon. Not. R. Astron. Soc., 404, 212-223 (2010)
	Constraints on star-forming galaxies at z ≥ 6.5 from HAWK-I Y-band imaging of GOODS-south.
o	Tables 1-2: <[HBJ2010] NNNN> N=4+4. Paragr. 3.3: <[HBJ2010] JHHMMSS.s+DDMMSS.s>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBJ2016]
[HBJ2016]	(Hendricks+Boeche+Johnson+, 2016)
Write:	<<[HBJ2016] rNNNN>> <<[HBJ2016] bNNNN>> <<[HBJ2016] r_NNNN>> (not recognised by Simbad, but found in literature) <<[HBJ2016] b_NNNN>>
N:	15+15
Object:	* (SIMBAD class: Star)
Note:	Las Campana Magellan 6.5m Clay telescope Michigan/Magellan Fiber System spectroscopy of N=15+15 stars in the Fornax H4 globular cluster. Use of archival HST imaging data.
in source:	NAME Fornax H4
Ref:	=2016A&A...585A..86H
by	HENDRICKS B. , BOECHE C., JOHNSON C.I., FRANK M.J., KOCH A., MATEO M., BAILEY III J.I.
	Astron. Astrophys., 585A, 86-86 (2016)
	Evidence for a chemical enrichment coupling of globular clusters and field stars in the Fornax dSph.
o	Tables A.1-A.3: <[HBJ2016] rNNNN> N=15 among (Nos 6-24), <[HBJ2016] bNNNN> N=15 among (Nos 1-23).
=E=	Catalogue in electronic form as J/A+A/585/A86
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HBK
HBK	(Huchra+Brodie+Kent)
Write:	<<HBK NNN-NNN>>
N:	150+21
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	Table 1: The format is a combination of the designations given by Battistini+ 1980 (acronyme Bol) and by Sargent+ 1977 (acronyme SKHB). For ex., '291-9' is Bol 291 and SKHB 9. Table 2: 17 Galaxies, 3 stars, 1 HII region
in source:	M 31 = NGC 224
Ref:	=1991ApJ...370..495H
by	HUCHRA J.P. , BRODIE J.P., KENT S.M.
	Astrophys. J., 370, 495-504 (1991)
	Extragalactic globular cluster. II. The M 31 globular cluster system.
o	HBK 4-000 is HBK 4-50
o	Table 1: <HBK NNN-NNN> N=150. Combination of Bol and SKHB
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HBK2008]
[HBK2008]	(Hennemann+ Birkmann+Krause+, 2008)
Write:	<<[HBK2008] JHHMMm+DDMM SMMN W>> <<[HBK2008] JHHMMm+DDMM IR N>>
N:	3+3+1+3+2
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	JCMT SCUBA observations of N=5 ISOSS sources.
in source:	ISOSS J19357+1950
in source:	ISOSS J19486+2556
in source:	ISOSS J20153+3453
in source:	ISOSS J20298+3559
in source:	ISOSS J22478+6357
Ref:	=2008A&A...485..753H
by	HENNEMANN M. , BIRKMANN S.M., KRAUSE O., LEMKE D.
	Astron. Astrophys., 485, 753-763 (2008)
	An infrared-submillimeter study of starforming regions selected by the ISOSS 170 µm survey.
o	Figure 6 ISOSS J19357+2556 is a misprint for ISOSS J19357+1950.
o	Table 2, Figs: <[HBK2008] JHHMMm+DDMM SMMN W> N=3+3+1+3+2. Figs 1-5: <[HBK2008] JHHMMm+DDMM IR N> N=5+4+2+8+8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBK2009]
[HBK2009]	(Heesen+Beck+Krause+, 2009)
Write:	<<[HBK2009] N>>
N:	8
Object:	(Radio) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 3.6cm, 6.2cm, 20cm, and 90cm continuum observations of NGC 253.
in source:	NGC 253
Ref:	=2009A&A...494..563H
by	HEESEN V. , BECK R., KRAUSE M., DETTMAR R.-J.
	Astron. Astrophys., 494, 563-577 (2009)
	Cosmic rays and the magnetic field in the nearby starburst galaxy NGC253. I. The distribution and transport of cosmic rays.
o	Table 2, Fig. 4-7: <[HBK2009] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBK96]
[HBK96]	(Hogg+Blandford+Kundic+, 1996)= (HDF)
Write:	<<[HBK96] JHHMMSS+DDMMSS>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Hubble Deep Field survey: N=2 candidate gravitational lenses.
in source:	NAME HDFN
Ref:	=1996ApJ...467L..73H
by	HOGG D.W. , BLANDFORD R., KUNDIC T., FASSNACHT C.D., MALHOTRA S.
	Astrophys. J., 467, 73-76 (1996)
	A candidate gravitational lens in the Hubble Deep Field.
o	<[HBK96] JHHMMSS+DDMMSS> N=2
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBL2004]
[HBL2004]	(Harman+Bryce+Lopez+, 2004) (Not yet in Simbad)
Write:	<<[HBL2004] KNw>>
N:	3+5
Object:	Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Knots of bright emission in the PN G190.3-17.7. Some are in pairs (K1s-K1n, K2s-K2n).
in source:	PN G190.3-17.7
Ref:	=2004MNRAS.348.1047H
by	HARMAN D.J. , BRYCE M., LOPEZ J.A., MEABURN J., HOLLOWAY A.J.
	Mon. Not. R. Astron. Soc., 348, 1047-1054 (2004)
	J320 (PN G190.3-17.7) as a poly-polar planetary nebula surrounded by point-symmetric knots.
o	Fig.2, Table 2: <[HBL2004] KNw> (Nos K1-K3, K1s, K1n, K2s, K2n, K3w).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBL2016]
[HBL2016]	(Huang+Bradac+Lemaux+, 2016)
Write:	<<[HBL2016] MACS HHMM-NNNN>> <<[HBL2016] RXJ HHMM-NNNN>> <<[HBL2016] RCS 2327-1282>>
N:	10+3+1
Object:	G (SIMBAD class: Galaxy)
Note:	HST WFC3 NIR observations of Spitzer IRAC-detected 6≲z≲10 galaxy candidates from the Spitzer UltRa Faint SUrvey Program (SURFS UP). Use of CLASH data.
Ref:	=2016ApJ...817...11H
by	HUANG K.-H. , BRADAC M., LEMAUX B.C., RYAN R.E.Jr, HOAG A., CASTELLANO M., AMORIN R., FONTANA A., BRAMMER G.B., CAIN B., LUBIN L.M., MERLIN E., SCHMIDT K.B., SCHRABBACK T., TREU T., GONZALEZ A.H., VON DER LINDEN A., KNIGHT R.I.
	Astrophys. J., 817, 11 (2016)
	Spitzer UltRa faint SUrvey program (SURFS UP). II. IRAC-detected lyman-break galaxies at 6 ≲ z ≲ 10 behind strong-lensing clusters.
o	Figs 4-5, Table 3: <[HBL2016] MACS HHMM-NNNN> N=11, <[HBL2016] RXJ HHMM-NNNN> N=3, <[HBL2016] RCS 1327-1282> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBM2005]
[HBM2005]	(Hill+Burton+Minier+, 2005)
Write:	<<[HBM2005] GLLL.lll+BB.bbb>> <<[HBM2005] GLLL.lll+BB.bbbA>> <<[HBM2005] GLLL.lll+BB.bbba>>
N:	404+2+11
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	SEST SIMBA 1.2 mm continuum observations of massive star formation regions. See also [HTB2006]
Ref:	=2005MNRAS.363..405H
by	HILL T. , BURTON M.G., MINIER V., THOMPSON M.A., WALSH A.J., HUNT-CUNNINGHAM M., GARAY G.
	Mon. Not. R. Astron. Soc., 363, 405-451 (2005)
	Millimetre continuum observations of southern massive star formation regions - I. SIMBA observations of cold cores.
o	Table 5: <[HBM2005] GLLL.lll+BB.bbb>, <[HBM2005] GLLL.lll+BB.bbbA>, <[HBM2005] GLLL.lll+BB.bbba>, N=404.
Ref:	=2006MNRAS.368.1223H
by	HILL T. , THOMPSON M.A., BURTON M.G., WALSH A.J., MINIER V., CUNNINGHAM M.R., PIERCE-PRICE D.
	Mon. Not. R. Astron. Soc., 368, 1223-1268 (2006)
	Millimetre continuum observations of southern massive star formation regions - II. SCUBA observations of cold cores and the dust grain emissivity index (β).
o	Table 3: <[HTB2006] GLLL.ll+BB.bb>, <[HTB2006] GLLL.lll+BB.bbb>, N=212. Table 4: <[HBM2005] GLLL.lll+BB.bbb> N=2 added.
Ref:	=2009MNRAS.392..768H
by	HILL T. , PINTE C., MINIER V., BURTON M.G., CUNNINGHAM M.R.
	Mon. Not. R. Astron. Soc., 392, 768-782 (2009)
	Spectral energy distribution modelling of southern candidate massive protostars using the Bayesian inference method.
o	Table 2: <[HBM2005] GLLL.lll+BB.bbb> N=11 added.
=E=	Catalogue in electronic form as J/MNRAS/363/405
=E=	Catalogue in electronic form as J/MNRAS/368/1223
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBM2006]
[HBM2006]	(Hachisuka+Brunthaler+Menten+, 2006)= ([HBM2006a]) (Not yet in Simbad)
Write:	<<[HBM2006] NN>>
N:	42
Object:	H2O Maser (SIMBAD class: Maser)
Note:	VLBA observations of H2O masers in the region W 3(OH).
in source:	W 3:W 3(OH) = W 3(OH)
Ref:	=2006ApJ...645..337H
by	HACHISUKA K. , BRUNTHALER A., MENTEN K.M., REID M.J., IMAI H., HAGIWARA Y., MIYOSHI M., HORIUCHI S., SASAO T.
	Astrophys. J., 645, 337-344 (2006)
	Water maser motions in W3(OH) and a determination of its distance.
o	Table 2: <[HBM2006] NN> (Nos 1-42).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBM2006a]
[HBM2006a]	(Hachisuka+Brunthaler+Menten+, 2006) (Not yet in Simbad)
*****	Avoid the usage of [HBM2006a], prefer [HBM2006]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBM2006b]
[HBM2006b]	(Hunter+Brogan+Megeath+, 2006)= (SMA)
Write:	<<[HBM2006b] I-SMAN>> <<[HBM2006b] I(N)-SMANNa>>
N:	4+7+3+1+16
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Submillimeter Array (SMA) 1.3mm continuum emission of the 2 NGC 6334 regions MFSW I and MFSW I(N).
in source:	NGC 6334:MFSW I = MFSW I
in source:	NGC 6334:MFSW I(N) = MFSW I(N)
Ref:	=2006ApJ...649..888H
by	HUNTER T.R. , BROGAN C.L., MEGEATH S.T., MENTEN K.M., BEUTHER H., THORWIRTH S.
	Astrophys. J., 649, 888-893 (2006)
	Millimeter multiplicity in NGC 6334 I and I(N).
o	Table 1: <[HBM2006b] I-SMAN> (Nos I-SMA1 to I-SMA4), <[HBM2006b] I(N)-SMAN> (Nos I(N)-SMA1 to I(N)-SMA7).
Ref:	=2007ApJ...654L.143R
by	RODRIGUEZ L.F. , ZAPATA L.A., HO P.T.P.
	Astrophys. J., 654L, 143-146 (2007)
	Compact centimeter and millimeter sources in NGC 6334 I(N): OB stars in the making?
o	Parag. 2 : Calibrator 1720-358 not identified
o	Tables 1, 2, Fig.3: <[HBM2006b] I(N)-SMA1a> (Nos SMA1a to SMA1c) added. Table 1: <[RZH2007] VLA-KN> (No. K1).
Ref:	=2009ApJ...707....1B
by	BROGAN C.L. , HUNTER T.R., CYGANOWSKI C.J., INDEBETOUW R., BEUTHER H., MENTEN K.M., THORWIRTH S.
	Astrophys. J., 707, 1-23 (2009)
	Digging into NGC 6334 I(N): multiwavelength imaging of a massive protostellar cluster.
o	Calibrator J1720-355 is not in SIMBAD.
o	Table 1: <[BHC2009] VLAN> (No. VLA3), <[HBM2006b] I(N)-SMANa> (No. SMA1d) added.
Ref:	=2014ApJ...788..187H
by	HUNTER T.R. , BROGAN C.L., CYGANOWSKI C.J., YOUNG K.H.
	Astrophys. J., 788, 187 (2014)
	Subarcsecond imaging of the NGC 6334 I(N) protocluster: two dozen compact sources and a massive disk candidate.
o	Table 2: <[HBM2006b] I(N)-SMANNa> N=16 (Nos I(N)-SMA8 to I(N)-SMA23) added. Table 3: <[HBC2014] VLA N> (No VLA 2), <[HBC2014] H2O-C4> N=1.
=E=	Catalogue in electronic form as <J/ApJ/707/1/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBM2011]
[HBM2011]	(Haines+Busarello+Merluzzi+, 2011)
Write:	<<[HBM2011] JHHMMSS.sss+DDMMSS.ss>>
N:	863
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spitzer MIPS observations of N=863 galaxies in the Shapley Supercluster. Use of optical SOS, UV GALEX, and IR UKIRT archival data.
in source:	NAME Shapley Concentration = NAME Shapley Supercluster
Ref:	=2011MNRAS.412..127H
by	HAINES C.P. , BUSARELLO G., MERLUZZI P., SMITH R.J., RAYCHAUDHURY S., MERCURIO A., SMITH G.P.
	Mon. Not. R. Astron. Soc., 412, 127-144 (2011)
	ACCESS – II. A complete census of star formation in the Shapley supercluster – UV and IR luminosity functions.
o	Table 1: <[HBM2011] JHHMMSS.sss+DDMMSS.ss> N=863.
=E=	Catalogue in electronic form as <J/MNRAS/412/127/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBM2012]
[HBM2012]	(HODGES-KLUCK+BREGMAN+MILLER+, 2012)= NGC891 ULX1
Write:	<<[HBM2012] NGC891 ULX1>>
N:	1 (SIMBAD class: ULX_Candidate = Ultra-luminous X-ray Source Candidate)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of a candidate ultraluminous source in NGC 891.
in source:	NGC 891
Ref:	=2012ApJ...747L..39H
by	HODGES-KLUCK E.J. , BREGMAN J.N., MILLER J.M., PELLEGRINI E.
	Astrophys. J., 747L, 39 (2012)
	A new ultraluminous X-ray source in the nearby edge-on spiral NGC 891.
o	<[HBM2012] NGC891 ULX1> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBM2016]
[HBM2016]	(Heywood+Bannister+Marvil+, 2016)
Write:	<<[HBM2016] JHHMMSS.ss+DDMMSS.ss>>
N:	3722
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ASKAP BETA (Boolardy Engineering Test Array) observations of N=3722 discrete radio components.
Ref:	=2016MNRAS.457.4160H
by	HEYWOOD I. , BANNISTER K.W., MARVIL J., ALLISON J.R., BALL L., BELL M.E., BOCK D.-J., BROTHERS M., BUNTON J.D., CHIPPENDALE A.P., COORAY F., CORNWELL T.J., DE BOER D., EDWARDS P., GOUGH R., GUPTA N., HARVEY-SMITH L., HAY S., HOTAN A.W., INDERMUEHLE B., JACKA C., JACKSON C.A., JOHNSTON S., KIMBALL A.E., KORIBALSKI B.S., LENC E., MACLEOD A., McCLURE-GRIFFITHS N., McCONNELL D., MIRTSCHIN P., MURPHY T., NEUHOLD S., NORRIS R.P., PEARCE S., POPPING A., QIAO R.Y., REYNOLDS J.E., SADLER E.M., SAULT R.J., SCHINCKEL A.E.T., SERRA P., SHIMWELL T.W., STEVENS J., TUTHILL J., TZIOUMIS A., VORONKOV M.A., WESTMEIER T., WHITING M.T.
	Mon. Not. R. Astron. Soc., 457, 4160-4178 (2016)
	Wide-field broad-band radio imaging with phased array feeds: a pilot multi-epoch continuum survey with ASKAP-BETA.
o	Table 3: <[HBM2016] JHHMMSS.ss+DDMMSS.ss> N=3722.
=E=	Catalogue in electronic form as <J/MNRAS/457/4160/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HBMR
HBMR	(Higgs+Broten+Medd+Raghavarao) (Not yet in Simbad)
Write:	<<HBMR NN>>
N:	31
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1964MNRAS.127..367H
by	HIGGS L.A. , BROTEN N.W., MEDD W.J., RAGHAVARAO R.
	Mon. Not. R. Astron. Soc., 127, 367-375 (1964)
	The Cygnus X complex.
o	Table 1: <HBMR NN> (Nos 1-31)
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [HBO96]
[HBO96]	(Hunter+Baum+O'Neil+, 1996)= ([HBO96a])
Write:	<<[HBO96] NNNNNN>>
N:	34484
Object:	* (SIMBAD class: Star)
Note:	HST WFPC2 observations. The format 'NNNNNN' is always a 6 digits format: 1st digit is the chip number, 2nd is the stellar-group number, the remaining 'NNNN' are a running identification number. Stars are ordered approximately by magnitude, from brightest to faintest. See also [HSH95] and [HBO96b]
in source:	NGC 604
Ref:	=1996ApJ...456..174H
by	HUNTER D.A. , BAUM W.A., O'NEIL E.J.Jr, LYNDS R.
	Astrophys. J., 456, 174-186 (1996)
	The intermediate stellar mass population in NGC 604 determined from Hubble Space Telescope images.
o	Clusters A to D are not objects, but different stellar groups (see p. 175)
o	Table 2: <[HBO96] NNNNNN> N=34484
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBO96a]
[HBO96a]	(Hunter+Baum+O'Neil+, 1996)
*****	Avoid the usage of [HBO96a], prefer [HBO96]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBO96b]
[HBO96b]	(Hunter+Baum+O'Neil+, 1996)
Write:	<<[HBO96b] NGC 206 NNNNNN>> <<[HBO96b] BF NNNNNN>>
N:	15379+20345
Object:	* (SIMBAD class: Star)
Note:	HST WFPC2 observations. The format 'NNNNNN' is always a 6 digits format. Table 2: * in NGC 206, format 'NGC 206 NNNNNN' N=15379. Table 3: * in Background Field, format 'BG NNNNNN', N=20345. 1st digit is the chip number, (Nos 1-4), the remaining 'NNNNN' are a running identification number. See also [HSH95] and [HBO96]
in source:	M 31:NGC 206 = NGC 206
Ref:	=1996ApJ...468..633H
by	HUNTER D.A. , BAUM W.A., O'NEIL E.J.Jr, LYNDS R.
	Astrophys. J., 468, 633-640 (1996)
	The intermediate stellar mass population in the M31 OB association NGC 206.
o	p.636 : OB78-3 = MAC OB 78-3
o	Table 2: <[HBO96b] NGC 206 NNNNNN> N=15379. Table 3: <[HBO96b] BF NNNNNN> N=20345
=E=	Catalogue in electronic form as J/ApJ/468/633
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HBQS
HBQS	(Homogeneous Bright QSO Survey)
Write:	<<HBQS HHMM+DDMMa>>
N:	565
Object:	QSO + G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	There is no format for objects in Table 4. The format 'HHMM+DDMM' (truncated coordinates) as given by the authors for QSOs is used in SIMBAD, with 'HHMM+DDMMa' for the few duplicated designations.
Ref:	=1995A&AS..112..347C
by	CRISTIANI S. , LA FRANCA F., ANDREANI P., GEMMO A., GOLDSCHMIDT P., MILLER L., VIO R., BARBIERI C., BODINI L., IOVINO A., LAZZARIN M., CLOWES R., MacGILLIVRAY H., GOUIFFES C., LISSANDRINI C., SAVAGE A.
	Astron. Astrophys., Suppl. Ser., 112, 347-366 (1995)
	The ESO key-programme "A homogeneous bright QSO survey". I. The methods and the "deep" fields.
o	Table 4: <HBQS HHMM+DDMMa> N=285
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HBR97]
[HBR97]	(Herbst+Beckwith+Robberto, 1997)
Write:	<<[HBR97] A>> <<[HBR97] SNN>>
N:	6+12
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=7 knots of H2 emission, (Nos A-F). N=12 other structures of H2 outflow, (Nos S1-S12). Maps in Figs 1, 2
in source:	NAME Serpens Cloud
Ref:	=1997ApJ...486L..59H
by	HERBST T.M. , BECKWITH S.V.W., ROBBERTO M.
	Astrophys. J., 486, 59-62 (1997)
	A new molecular hydrogen outflow in Serpens.
o	SMM-3= [CED93] 3
o	Table 1: <[HBR97] A> (Nos A-F), <[HBR97] SNN> (Nos S1-S12)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HBS
HBS	(Hintzen+Boeshaar+Scott)
*****	Avoid the usage of HBS, prefer [HBS81]
Origin	of the Acronym: L (1984ApJS...55..533H)
Details on Acronym: [HBS2006]
[HBS2006]	(Hartman+Bersier+Stanek+, 2006)
Write:	<<[HBS2006] NNNNNN>> <<[HBS2006] ext NNNNNN>>
N:	36709+59502
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	CFHT photometric observations of M 33.
in source:	M 33 = NGC 598
Ref:	=2006MNRAS.371.1405H
by	HARTMAN J.D. , BERSIER D., STANEK K.Z., BEAULIEU J.-P., KALUZNY J., MARQUETTE J.-B., STETSON P.B., SCHWARZENBERG-CZERNY A.
	Mon. Not. R. Astron. Soc., 371, 1405-1417 (2006)
	Deep Canada-France-Hawaii Telescope photometric survey of the entire M33 galaxy - I. Catalogue of 36000 variable point sources.
o	Table S1: <[HBS2006] NNNNNN> N=36709. Table S2: <[HBS2006] ext NNNNNN> N=59502.
=E=	Catalogue in electronic form as J/MNRAS/371/1405
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBS2013]
[HBS2013]	(Husband+Bremer+Stanway+, 2013)
Write:	<<[HBS2013] JHHMM+DDMM QSO NaNN>>
N:	13
Object:	LBG (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 observations of N=13 Lyman break galaxies (LBG) in the field of three QSOs (QSO J0338+0021, QSO J1204-0021, QSO J2130+0026).
Ref:	=2013MNRAS.432.2869H
by	HUSBAND K. , BREMER M.N., STANWAY E.R., DAVIES L.J.M., LEHNERT M.D., DOUGLAS L.S.
	Mon. Not. R. Astron. Soc., 432, 2869-2877 (2013)
	Are z ~ 5 quasars found in the most massive high-redshift overdensities ?
o	Table 4: <[HBS2013] JHHMM+DDMM QSO NaNN> N=13.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBS2015]
[HBS2015]	(Husband+Bremer+Stanway+, 2015)
Write:	<<[HBS2015] AN>> <<[HBS2015] AA>>
N:	22+12
Object:	G + LAE + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLT MUSE observations of N=22+12 galaxies, LAE, and stars in the field of the quasar PKS 1614+051. The format used here is an extension of the labelling scheme of Hu & Cowie (1987ApJ...317L...7H), see also [HC87].
Ref:	=2015MNRAS.452.2388H
by	HUSBAND K. , BREMER M.N., STANWAY E.R., LEHNERT M.D.
	Mon. Not. R. Astron. Soc., 452, 2388-2395 (2015)
	Dissecting the complex environment of a distant quasar with MUSE.
o	Sources A to I are from Hu & Cowie, 1987 ([HC87] sources in Simbad) except source G (not the same position).
o	Fig. 1, Table 1: <[HBS2015] AN> N=22 among (Nos A-B, E-I, J1-J2, L-O, P1-P2, Q-Z), <[HBS2015] AA> N=12 among (Nos AF-BN).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBS81]
[HBS81]	(Hintzen+Boeshaar+Scott, 1981)= (HBS)
Write:	<<[HBS81] 3C 275.1 NN>> <<[HBS81] 3C 270.1 NN>>
N:	37+15
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 1: objects in the field of the QSO 3C 275.1 and 3C 270.1. No. 1 is the QSO itself. See also [H84b]
Ref:	=1981ApJ...246L...1H
by	HINTZEN P. , BOESHAAR G.O., SCOTT J.S.
	Astrophys. J., 246, 1-4 (1981)
	Detection of an apparent, distant cluster of galaxies associated with the radio-tail QSO 3C 275.1.
o	Table 1: <[HBS81] 3C 275.1 NN> (Nos 1-37), <[HBS81] 3C 270.1 NN> (Nos 1-15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBS84]
[HBS84]	(Hill+Bohlin+Stecher, 1984)
Write:	<<[HBS84] NN>>
N:	76
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
in source:	M 101 = NGC 5457
Ref:	=1984ApJ...277..542H
by	HILL J.K. , BOHLIN R.C., STECHER T.P.
	Astrophys. J., 277, 542-549 (1984)
	Images in the rocket ultraviolet : photometry of M 101.
o	T.3: cross-id.: N = NGC, H = [H69] NGC 5457, S = [S71] M 101, AG = [AG79]
o	Table 2: <[HBS84] NN> (Nos 1-76)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBT2010]
[HBT2010]	(Haisch+Barsony+Tinney, 2010)
Write:	<<[HBT2010] NN>>
N:	22
Object:	T dwarf cand. (SIMBAD class: BrownD*_Candidate = Brown Dwarf Candidate)
Stat:	is completely incorporated in Simbad
Note:	AAT IRIS2 observations of N=22 T dwarf candidates in the ρ Oph cloud.
in source:	NAME rho Oph Cloud
Ref:	=2010ApJ...719L..90H
by	HAISCH K.E. , BARSONY M., TINNEY C.
	Astrophys. J., 719L, 90-94 (2010)
	A methane imaging survey for T dwarf candidates in ρ Ophiuchi.
o	Table 1: <[HBT2010] NN> (Nos 1-22).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBT2017]
[HBT2017]	(Hoag+Bradac+Trenti+, 2017)
Write:	<<[HBT2017] MACS1423-z7p64>>
N:	1
Object:	Grav. lensed image of a G (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck I MOSFIRE observations of N=1 galaxy, gravitationally magnified by the galaxy cluster MCS J1423.8+2404. Use of CLASH and GLASS data.
Ref:	=2017NatAs...1...91H
by	HOAG A. , BRADAC M., TRENTI M., TREU T., SCHMIDT K.B., HUANG K.-H., LEMAUX B.C., HE J., BERNARD S.R., ABRAMSON L.E., MASON C.A., MORISHITA T., PENTERICCI L., SCHRABBACK T.
	NatAs, 1, 91 (2017)
	Spectroscopic confirmation of an ultra-faint galaxy at the epoch of reionization.
o	<[HBT2017] MACS1423-z7p64> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HBV
HBV	(Hamburg-Bergedorf obs., Variable *)
Write:	<<*SV HBV** NNN>>
Object:	V* (1PN) (SIMBAD class: Variable* = Variable Star)
Note:	HBV 475 = V1329 Cyg = PK 077-05 1 (PN + M4+WN5 symbiotic *). see 1981SSRv...28..227V, p. 277. For the Magellanic Clouds, the HBV stars are identified in ref. 1967SAOP.4699....1H and 1977 Hodge+Wright Atlas of the SMC. See also LMV ref. 1970SAOSR.310....1G
Ref:	=1970ApL.....6....5C
by	CRAMPTON D. , GRYGAR J., KOHOUTEK L., VIOTTI R.
	Astrophys. Lett., 6, 5-None (1970)
	HBV 475: evolution stage of a planetary nebulae.
o	<SV* HBV NNN> (No. 475).
Details on Acronym: [HBV2021]
[HBV2021]	(Healy+Blyth+Verheijen+, 2021) (Not yet in Simbad)
Write:	<<[HBV2021] SNN>>
N:	15
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	N=15 groups of galaxies within the footprint of the Westerbork Coma Survey.
in source:	ACO 1656 = Coma Cluster
Ref:	=2021A&A...650A..76H
by	HEALY J. , BLYTH S.-L., VERHEIJEN M.A.W., HESS K.M., SERRA P., VAN DER HULST J.M., JARRETT T.H., YIM K., JOZSA G.I.G.
	Astron. Astrophys., 650A, 76-76 (2021)
	H I content in Coma cluster substructure.
o	Fig. 11, Table 2: <[HBV2021] SNN> (Nos S1-S15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HBW
HBW	(Hodge+Balsley+Wyder)
Write:	<<HBW NNNN>>
N:	1272
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Catalog of 1272 newly-recognized HII regions and compact emission regions in the galaxy M33, based on deep CCD images at H-alpha. This catalog does not include previously catalogued M33 HII regions as summarized by Courtes et al (1987A&A...174...28C) These objects will also be identified in Hodge, Skelton and Smith, an atlas of local group galaxies (Kluwer, Dordrecht) 1999.
in source:	M 33 = NGC 598
Ref:	=1999PASP..111..685H
by	HODGE P.W. , BALSLEY J., WYDER T.K., SKELTON B.P.
	Publ. Astron. Soc. Pac., 111, 685-690 (1999)
	The HII regions of M33. II. A photometric catalog of 1272 newly identified emission regions.
o	Table 1: <HBW NNNN> (Nos 1-1272).
=E=	Catalogue in electronic form as J/PASP/111/685
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [HBW2011]
[HBW2011]	(Hodge+Becker+White+, 2011)
Write:	<<[HBW2011] JHHMMSS.s+DDMMSS>>
N:	17969
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA 1.4GHz observations of N=17969 isolated radio components in the SDSS Stripe 82.
Ref:	=2011AJ....142....3H
by	HODGE J.A. , BECKER R.H., WHITE R.L., RICHARDS G.T., ZEIMANN G.R.
	Astron. J., 142, 3 (2011)
	High-resolution Very Large Array imaging of Sloan Digital Sky Survey Stripe 82 at 1.4 GHz.
o	Table 1: <[HBW2011] JHHMMSS.s+DDMMSS> N=17969.
=E=	Catalogue in electronic form as <J/AJ/142/3/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HBW98]
[HBW98]	(Hutchings+Baum+Weistrop+, 1998) (Not yet in Simbad)
Write:	<<[HBW98] 3C 135 A>> <<[HBW98] 3C 171 A>>
N:	10+6
Object:	Radio knot (SIMBAD class: PartofG = Part of a Galaxy)
Note:	HST spectrography of 3C galaxies.
in source:	3C 135
in source:	3C 171
Ref:	=1998AJ....116..634H
by	HUTCHINGS J.B. , BAUM S.A., WEISTROP D., NELSON C., KAISER M.E., GELDERMAN R.F.
	Astron. J., 116, 634-642 (1998)
	Spatially resolved spectra of 3C galaxy nuclei.
o	Fig.2: <[HBW98] 3C 135 A> 9Nos A-I, X), <[HBW98] 3C 171 A> (Nos A-E, X).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HC
HC	(Hillenbrand+Carpenter)
*****	Avoid the usage of HC, prefer [HC2000]
Origin	of the Acronym: L (2000AJ....120.1426G)
Details on Acronym: HC
HC	(Holden+Caswell)
*****	Avoid the usage of HC, prefer [HC69]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HC
HC	(Hartwick+Cowley)
*****	Avoid the usage of HC, prefer [HC88]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HC
HC	(Hofner+Churchwell)
*****	Avoid the usage of HC, prefer [HC96]
Origin	of the Acronym: L (1997A&A...327..299P)
Details on Acronym: HC
HC	(Hu+Cowie)
*****	Avoid the usage of HC, prefer [HCB2010]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HC
HC	(Heiles Cloud)
*****	Avoid the usage of HC, prefer HCl
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HC2000]
[HC2000]	(Hillebrand+Carpenter, 2000)= (HC)
Write:	<<[HC2000] NNN>>
N:	778
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	NAME ONC
Ref:	=2000ApJ...540..236H
by	HILLENBRAND L.A. , CARPENTER J.M.
	Astrophys. J., 540, 236-254 (2000)
	Constraints on the stellar/substellar mass function in the inner Orion nebula cluster.
o	Table 1: <[HC2000] NNN> (Nos 1-778, No. 187 missing).
=E=	Catalogue in electronic form as J/ApJ/540/236
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HC2005]
[HC2005]	(Hutawarakorn+Cohen, 2005)= ([HC2005a])
Write:	<<[HC2005] 1665-LHC A>> <<[HC2005] 1665-RHC a>> <<[HC2005] 1667-LHC A>> <<[HC2005] 1667-RHC a>> <<[HC2005] 1665 NN>> <<[HC2005] 1667 NN>>
N:	15+14+23+8+19+23
Object:	OH Maser (SIMBAD class: Maser)
Note:	MERLIN polarization measurements of OH 1665 and 1667 MHz masers in the star-forming region AFGL 2591.
in source:	RAFGL 2591
Ref:	=2005MNRAS.357..338H
by	HUTAWARAKORN B. , COHEN R.J.
	Mon. Not. R. Astron. Soc., 357, 338-344 (2005)
	OH maser disc and magnetic field structure in AFGL 2591.
o	Table 1: <[HC2005] 1665-LHC A> (Nos A-O), <[HC2005] 1665-RHC a> (Nos a-n), <[HC2005] 1667-LHC A> (Nos A-W), <[HC2005] 1667-RHC a> (Nos a-h). Table 2: <[HC2005] 1665 NN> (Nos 1-19), <[HC2005] 1667 NN> (Nos 1-23).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HC2005a]
[HC2005a]	(Hutawarakorn+Cohen, 2005) (Not yet in Simbad)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HC2005b]
[HC2005b]	(HArvey-Smith+Cohen, 2005)
Write:	<<[HC2005b] JHHMMSS.ssss+DDMMSS.sss>> <<[HC2005b] JHHMMSS.ss+DDMMSS.ss>> <<[HC2005b] JHHMMSS.ss+DDMMSS.s>>
N:	22
Object:	OH Maser (SIMBAD class: Maser)
Note:	MERLIN observations of OH emission in star-forming regions.
Ref:	=2005MNRAS.356..637H
by	HARVEY-SMITH L. , COHEN R.J.
	Mon. Not. R. Astron. Soc., 356, 637-646 (2005)
	A MERLIN survey of 4.7-GHz excited OH masers in star-forming regions.
o	Table 2: <[HC2005b] JHHMMSS.ssss+DDMMSS.sss>, <[HC2005b] JHHMMSS.ss+DDMMSS.ss>, <[HC2005b] JHHMMSS.ss+DDMMSS.s>, N=22.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HC2006]
[HC2006]	(Hadfield+Crowther, 2006)
Write:	<<[HC2006] AN>>
N:	4
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	Star clusters in the regions [SCK99] NGC 3125 A and B. Use of archival HST STIS and FOC data. See also [SSC2006].
in source:	NGC 3125
Ref:	=2006MNRAS.368.1822H
by	HADFIELD L.J. , CROWTHER P.A.
	Mon. Not. R. Astron. Soc., 368, 1822-1832 (2006)
	How extreme are the Wolf-Rayet clusters in NGC 3125?
o	NGC 3125-A, B = [SCK99] NGC 3125 A, B
o	Figs 3, 4: <[HC2006] AN> (Nos A1-A2, B1-B2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HC2007]
[HC2007]	(Hadfield+Crowther, 2007)
Write:	<<[HC2007] HN>> <<[HC2007] NN>>
Object:	HII + Poss. WR* (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS1 survey of NGC 1313.
in source:	NGC 1313
Ref:	=2007MNRAS.381..418H
by	HADFIELD L.J. , CROWTHER P.A.
	Mon. Not. R. Astron. Soc., 381, 418-432 (2007)
	A survey of the Wolf-Rayet population of the barred, spiral galaxy NGC 1313.
o	Table 4: <[PES80] NN> (No. 12) added. Table A1: <[HC2007] HN> (Nos H1-H9). Table A2: <[HC2007] NN> (Nos 1-94).
=E=	Catalogue in electronic form as J/MNRAS/381/418
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HC2009]
[HC2009]	(Hwang+Chang, 2009)= ([HC2009a])
Write:	<<[HC2009] NNNNN>>
N:	15147
Object:	Pair of G (SIMBAD class: PairG = Pair of Galaxies)
Note:	New catalog and images of interacting and merging galaxies from CFHT observations.
Ref:	=2009ApJS..181..233H
by	HWANG C.-Y. , CHANG M.-Y.
	Astrophys. J., Suppl. Ser., 181, 233-237 (2009)
	A catalog of morphologically identified merging galaxies.
o	Table 1: <[HC2009] NNNNN> (Nos 1-15147).
=E=	Catalogue in electronic form as J/ApJS/181/233
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HC2009a]
[HC2009a]	(Hwang+Chang, 2009)
*****	Avoid the usage of [HC2009a], prefer [HC2009]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HC2009b]
[HC2009b]	(Herrmann+Ciardullo, 2009)
Write:	<<[HC2009b] IC 342-NNN>> <<[HC2009b] M74-NNN>> <<[HC2009b] M83-NNN>> <<[HC2009b] M94-NNN>> <<[HC2009b] M101-NN>> <<[HC2009b] NGC 5068-NN>> <<[HC2009b] NGC 6946-NN>>
N:	165+153+241+150+65+19+71
Object:	PN + Poss. PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	WIYN/Hydra, CTIO Blanco/Hydra and HET/MRS spectroscopy of nearby galaxies.
in source:	IC 342
in source:	M 74 = NGC 628
in source:	M 83 = NGC 5236
in source:	M 94
in source:	M 101 = NGC 5457
in source:	NGC 5068
in source:	NGC 6946
Ref:	=2009ApJ...703..894H
by	HERRMANN K.A. , CIARDULLO R.
	Astrophys. J., 703, 894-904 (2009)
	Planetary nebulae in face-on spiral galaxies. II. Planetary nebula spectroscopy.
o	Table 4: <[HC2009b] IC 342-NNN> (Nos 1-165), <[HC2009b] M74-NNN> (Nos 1-153), <[HC2009b] M83-NNN> (Nos 1-241), <[HC2009b] M94-NNN> (Nos 1-150), <[HC2009b] M101-NN> (Nos 1-65). Table 6: <[HC2009b] NGC 5068-NN> (Nos 1-19). Table 7: <[HC2009b] NGC 6946-NN> (Nos 1-71).
=E=	Catalogue in electronic form as <J/ApJ/703/894/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HC2011]
[HC2011]	(Hankey+Cole, 2011)
Write:	<<[HC2011] NNNN>>
N:	43
Object:	RGB* (SIMBAD class: RGB* = Red Giant Branch star)
Note:	AAT AAOmega spectroscopic observations of the globular cluster IC 4499. Use of 2MASS data.
in source:	IC 4499
Ref:	=2011MNRAS.411.1536H
by	HANKEY W.J. , COLE A.A.
	Mon. Not. R. Astron. Soc., 411, 1536-1546 (2011)
	Radial velocity and metallicity of the globular cluster IC4499 obtained with AAOmega.
o	Table 3: <[HC2011] NNNN> N=43 among (Nos 4976-7910).
=E=	Catalogue in electronic form as J/MNRAS/411/1536
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HC2014]
[HC2014]	(Hayashi+Chiba, 2014)
Write:	<<[HC2014] NN>>
N:	91
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	N=91 globular clusters in the halo of M 31.
in source:	M 31 = NGC 224
Ref:	=2014ApJ...789...62H
by	HAYASHI K. , CHIBA M.
	Astrophys. J., 789, 62 (2014)
	The prolate dark matter halo of the Andromeda galaxy.
o	Table 1: <[HC2014] NN> (Nos 1-91).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HC69]
[HC69]	(Holden+Caswell, 1969)= (HC)
Write:	<<[HC69] NN>>
N:	45
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Ref:	=1969MNRAS.143..407H
by	HOLDEN D.J. , CASWELL J.L.
	Mon. Not. R. Astron. Soc., 143, 407-435 (1969)
	178 MHz observations of galactic radio sources.
o	Table III: <[HC69] NN> (Nos 1-45)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HC73]
[HC73]	(Haro+Chavira, 1973)= (HFS) = ([PCG94a])
Write:	<<[HC73] NN>>
N:	14
Object:	Flare * (SIMBAD class: Eruptive* = Eruptive Variable)
Stat:	is completely incorporated in Simbad
Note:	Second ref. continues the numbering of [HC73] for (Nos 8-14). In SIMBAD, all objects are '[HC73] NN' objects.
in source:	NAME ASS CYG T 1-
Ref:	=1973BITon...1...17H
by	HARO G. , CHAVIRA E.
	Bol. Inst. Tonantzintla, 1, 17-21 (1973)
	Anote on some flare stars in Cygnus.
o	<[HC73] N> N=7
Ref:	=1994IBVS.4046....1P
by	PARSAMIAN E.S. , CHAVIRA E., GONZALEZ G.
	IAU Inform. Bull. Var. Stars, 4046, 1-2 (1994)
	New flare stars in the Cygnus T1 association region.
o	<[HC73] NN> (Nos 8-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HC74]
[HC74]	(Haro+Chavira, 1974)= (HFS) = ([PCG94b])
Write:	<<[HC74] N>>
N:	8
Object:	Flare * (SIMBAD class: Eruptive* = Eruptive Variable)
Stat:	is completely incorporated in Simbad
Note:	Second ref. continues the numbering of [HC74] for (Nos 5-8). In SIMBAD, all objects are '[HC74] N' objects.
in source:	NAME Ophiuchus Region
in source:	NAME Sco Region
Ref:	=1974BITon...1..189H
by	HARO G. , CHAVIRA E.
	Bol. Inst. Tonantzintla, 1, 189-192 (1974)
	A note on some flare stars in Ophiuchus ans Scorpius.
o	<[HC74] N> N=4
Ref:	=1994IBVS.4047....1P
by	PARSAMIAN E.S. , CHAVIRA E., GONZALEZ G.
	IAU Inform. Bull. Var. Stars, 4047, 1-2 (1994)
	New flare stars in the region of Ophiuchus and Scorpius.
o	<[HC74] N> (Nos 5-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HC86]
[HC86]	(Hester+Cox, 1986)
Write:	<<[HC86] XA>> <<[HC86] Knot>>
N:	3+1
Object:	(X) + Knot (SIMBAD class: PartofCloud = Part of Cloud)
Note:	Einstein HRI observations. N=3 X-ray sources (Nos XA-XC) and N=1 Knot.
in source:	X Cyg X-5
Ref:	=1986ApJ...300..675H
by	HESTER J.J. , COX D.P.
	Astrophys. J., 300, 675-697 (1986)
	The Cygnus Loop : a detailed comparison of X-ray and optical emission.
o	Fig.4: Others features than [HC86] designations are not in SIMBAD.
o	Fig.4: <[HC86] XA> (Nos XA-XC), <[HC86] Knot> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HC87]
[HC87]	(Hu+Cowie, 1987)
Write:	<<[HC87] PKS 1614A>>
N:	10
Object:	? + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	CFHT broad- and narrow-band observations of N=1 companion of PKS 1614+051 and N=9 galaxies in the field of PKS 1614+051.
Ref:	=1987ApJ...317L...7H
by	HU E.M. , COWIE L.L.
	Astrophys. J., 317, 7-12 (1987)
	The distribution of gas and galaxies around the distant quasar PKS 1614+051.
o	Fig. 1, Table 2: <[HC87] PKS 1614A> (Nos A-J).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HC88]
[HC88]	(Hartwick+Cowley, 1988)= (CH) = (HC) = (LMC CH)
Write:	<<[HC88] NNN>>
N:	53
Object:	CH * (SIMBAD class: Star)
Note:	N=53 among (Nos 1-222)
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1988ApJ...334..135H
by	HARTWICK F.D.A. , COWLEY A.P.
	Astrophys. J., 334, 135-143 (1988)
	The kinematics of an old stellar population in the Large Magellanic Cloud : the CH stars.
o	<[HC88] NNN> N=53 among (Nos 1-222)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HC89]
[HC89]	(Helfand+Chanan, 1989)
Write:	<<[HC89] NN>>
N:	47
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Ref:	=1989AJ.....98.1652H
by	HELFAND D.J. , CHANAN G.A.
	Astron. J., 98, 1652-1658 (1989)
	A search for X-ray counterparts to small-diameter galactic radio sources.
o	Table I: <[HC89] NN> N=47
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HC93]
[HC93]	(He+Chen, 1993)
Write:	<<[HC93] HHMMm+DDMMA>>
N:	348
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Note:	Finding charts of N=348 QSOs candidates (1993), catalogue with positions (1998).
Ref:	=1993Ap&SS.200..279H
by	HE R. , CHEN J.-S.
	Astrophys. Space Sci., 200, 279-311 (1993)
	Objective prism survey of QSOs in the field centered at 10h40m +00 00'.
o	<[HC93] HHMMm+DDMMA> N=348.
Ref:	=1998PBeiO..32...15H
by	HE R. , CHEN J.-S.
	Publ. Beijing Astron. Obs., 32, 15-24 (1998)
	Objective prism survey of QSOs in the field centered at 10h 40m + 00 °. 00 '.
o	Table 2: <[HC93] HHMMm+DDMMA> N=348.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HC96]
[HC96]	(Hofner+Churchwell, 1996)= (HC)
Write:	<<[HC96] GLL.ll+B.bb>> <<[HC96] GLL.ll+B.bb NN>>
N:	21+109
Object:	HII + H2O Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	Table 3: N=109 H2O maser features format 'GLL.ll+B.bb NN' in the 21 HII regions format 'GLL.ll+B.bb' (Table 2).
Ref:	=1996A&AS..120..283H
by	HOFNER P. , CHURCHWELL E.
	Astron. Astrophys., Suppl. Ser., 120, 283-299 (1996)
	A survey of water maser emission toward ultracompact HII regions.
o	Table 2: 43.89-0.38 misprint for 43.89-0.78?
o	Table 2: <[HC96] GLL.ll+B.bb> N=21. Table 3: <[HC96] GLL.ll+B.bb NN> N=109
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCA99]
[HCA99]	(Hartmann+Calvet+Allen+, 1999)
Write:	<<[HCA99] A>> <<[HCA99] A/B>>
N:	4
Object:	Knot (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	HST near-IR NICMOS observations of IRAS 04325+2402. N=3 knots, the 2 knots A and B are associated in a same object 'A/B'.
in source:	IRAS 04325+2402
Ref:	=1999AJ....118.1784H
by	HARTMANN L. , CALVET N., ALLEN L., CHEN H., JAYAWARDHANA R.
	Astron. J., 118, 1784-1790 (1999)
	The complex protostellar source IRAS 04325+2402.
o	Table 1: <[HCA99] A> (Nos A-C), <[HCA99] A/B> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCB2002]
[HCB2002]	(Hutawarakorn+Cohen+Brebner, 2002)
Write:	<<[HCB2002] HHMMSS.ss+DDMMSS.s>> <<[HCB2002] HHMMSS.sss+DDMMSS.ss>>
N:	7
Object:	OH Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
in source:	W 75:W 75N = W 75N
Ref:	=2002MNRAS.330..349H
by	HUTAWARAKORN B. , COHEN R.J., BREBNER G.C.
	Mon. Not. R. Astron. Soc., 330, 349-364 (2002)
	OH masers and magnetic fields in the bipolar outflow source W75N.
o	Table 2: <[HCB2002] HHMMSS.ss+DDMMSS.s>, <[HCB2002] HHMMSS.sss+DDMMSS.ss>, N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCB2006]
[HCB2006]	(Halliday+Carter+Bridges+, 2006)
Write:	<<[HCB2006] FD-NN-N-NN>> <<[HCB2006] PN-NN-N-NNN>>
N:	40+442
Object:	* + PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat.	in SIMBAD: PNe (Table A1) are completely incorporated.
Note:	Sample of PNs using the WYFFOS fibre spectrograph on the William Herschel Telescope. 40 fiducial (FD in the format) standard stars are used.
in source:	M 31 = NGC 224
Ref:	=2006MNRAS.369...97H
by	HALLIDAY C. , CARTER D., BRIDGES T.J., JACKSON Z.C., WILKINSON M.I., QUINN D.P., EVANS N.W., DOUGLAS N.G., MERRETT H.R., MERRIFIELD M.R., ROMANOWSKY A.J., KUIJKEN K., IRWIN M.J.
	Mon. Not. R. Astron. Soc., 369, 97-119 (2006)
	Planetary nebula velocities in the disc and bulge of M31.
o	Table 1: <[HCB2006] FD-NN-N-NN> N=40. Table A1: <[HCB2006] PN-NN-N-NNN> N=442.
=E=	Catalogue in electronic form as J/MNRAS/369/97
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCB2007]
[HCB2007]	(Hernandez+Calvet+Briceno+, 2007)
Write:	<<[HCB2007] OB1a NNNN>>
N:	115+106+41+65
Object:	*iA (SIMBAD class: Star)
Note:	Spitzer observations of 2 fields in Orion OB 1 association. See also CVSO.
in source:	NAME ASS ORI OB 1-
Ref:	=2007ApJ...671.1784H
by	HERNANDEZ J. , CALVET N., BRICENO C., HARTMANN L., VIVAS A.K., MUZEROLLE J., DOWNES J., ALLEN L., GUTERMUTH R.
	Astrophys. J., 671, 1784-1799 (2007)
	Spitzer observations of the Orion OB1 association: disk census in the low-mass stars.
o	Tables 1, 3: <[HCB2007] OB1a NNNN> N=115+41 among (Nos 9-1861). Tables 2, 4: <[HCB2007] OB1b NNNN> N=106+65 among (Nos 21-2386).
=E=	Catalogue in electronic form as J/ApJ/671/1784
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCB2010]
[HCB2010]	(Hu+Cowie+Barger+, 2010)= (HC)
Write:	<<[HCB2010] NB816 NN>> <<[HCB2010] NB921 N>> <<[HCB2010] HC JHHMMSS+DDMMSS>> <<[HCB2010] HCHHMMSS+DDMMSS>> (not recognised by Simbad, but found in literature)
N:	12+4+118
Object:	Poss. LAE + LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Subaru Suprime-Cam (NB816 and NB921) and Keck II DEIMOS observations of candidate Lyman α emitters.
in source:	NAME GOODS North Field
Ref:	=2010ApJ...725..394H
by	HU E.M. , COWIE L.L., BARGER A.J., CAPAK P., KAKAZU Y., TROUILLE L.
	Astrophys. J., 725, 394-423 (2010)
	An atlas of z = 5.7 and z = 6.5 Lyα emitters.
o	48 HC names in the SSA22 fields were originally written with a minus sign, but all sources of these fields have a positive J2000 declination
o	Table 2: <[HCB2010] NB816 NN> (Nos 1-12). Table 3: <[HCB2010] NB921 NN> (Nos 1-4). Tables 5-7: <[HCB2010] HC JHHMMSS+DDMMSS> N=88+27+3.
=E=	Catalogue in electronic form as <J/ApJ/725/394/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCB2017]
[HCB2017]	(Hsu+Cowie+Barger+, 2017)
Write:	<<[HCB2017] SMA-N>> <<[HCB2017] SMA-N-N>>
N:	6+4
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SMA observations of N=6+4 submillimeter sources for six SCUBA-2 850µm sources in five lensing cluster fields.
in source:	ACO 1689
in source:	ACO 2390
in source:	ACO 370
in source:	ClG J0717+3745 = MCS J0717.5+3745
in source:	ClG J1423+2404 = MCS J1423.8+2404
Ref:	=2017ApJ...850..189H
by	HSU L.-Y. , COWIE L.L., BARGER A.J., WANG W.-H.
	Astrophys. J., 850, 189-189 (2017)
	The Hawaii SCUBA-2 Lensing Cluster Survey: are low-luminosity submillimeter galaxies detected in the rest-frame UV?
o	Fig. 1, Table 4: <[HCB2017] SMA-N> (Nos 1-6), <[HCB2017] SMA-N-N> (Nos 2-1 to 2-2, 3-1 to 3-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCB95]
[HCB95]	(Hill+Cheng+Bohlin+, 1995)
Write:	<<[HCB95] LH 52 NNNN>> <<[HCB95] LH 53 NNNN>>
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Note:	Table 2: 10 brightest UV sources in LH 52, format 'LH 52 NNNN'. Table 3: 10 brightest UV sources in LH 53, format 'LH 53 NNNN'. Observations with the UIT telescope aboard Astro-1 Space Shuttle Mission
in source:	LH 52
in source:	LH 53
Ref:	=1995ApJ...446..622H
by	HILL R.S. , CHENG K.-P., BOHLIN R.C., O'CONNELL R.W., ROBERTS M.S., SMITH A.M., STECHER T.P.
	Astrophys. J., 446, 622-636 (1995)
	UIT and optical imagery of Large Magellanic Cloud associations LH 52 and LH 53: ages and initial mass function slopes.
o	Table 2: <[HCB95] LH 52 NNNN>, Table 3: <[HCB95] LH 53 NNNN>
=E=	Catalogue in electronic form as J/ApJ/446/622
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCB98]
[HCB98]	(Hogg+Cohen+Blandford+, 1998)= (H) = (HDF)
Write:	<<[HCB98] HMMSSs-MMSS>>
N:	27
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Observations of the Hubble Deep Field. In the format the letter 'H' stands for HDF, 'MMSS.s-MMSS', relative to 12h and +62deg. See also [CCH96].
in source:	NAME HDFN
Ref:	=1998AJ....115.1418H
by	HOGG D.W. , COHEN J.G., BLANDFORD R., GWYN S.D.J., HARTWICK F.D.A., MOBASHER B., MAZZEI P., SAWICKI M., LIN H., YEE H.K.C., CONNOLLY A.J., BRUNNER R.J., CSABAI I., DICKINSON M., SUBBARAO M.U., SZALAY A.S., FERNANDEZ-SOTO A., LANZETTA K.M., YAHIL A.
	Astron. J., 115, 1418-1422 (1998)
	A blind test of photometric redshift prediction.
o	HH = 12h, DD = +62°
o	Table 1: <[HCB98] AMMSSs-MMSS> N=27
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HCC
HCC	(Hydra I Cluster Catalogue)
Write:	<<HCC NNN>>
N:	111
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS1 observations of the Hydra I Cluster.
in source:	NAME Hya I Cluster
Ref:	=2008A&A...486..697M
by	MISGELD I. , MIESKE S., HILKER M.
	Astron. Astrophys., 486, 697-709 (2008)
	The early-type dwarf galaxy population of the Hydra I cluster.
o	Table 2: <[MMH2008] Na-NN> (No. 7a-31),<[MMH2008] aN-NN> (Nos q2-15, q3-18). Table A2: <HCC NNN> (Nos 1-111).
=E=	Catalogue in electronic form as J/A+A/486/697
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCC2001]
[HCC2001]	(Haines+Clowes+Campusano+, 2001)
Write:	<<[HCC2001] CN>> <<[HCC2001] GN>> <<[HCC2001] Cluster A>> <<[HCC2001] NN>>
N:	4+3+2+18
Object:	G + Cluster of G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Study of the galaxy environment of QSO 1044+059. Fig.5: brightest galaxies (Nos G1-G4, C1-C3). Fig.6, Table 3: N=2 clusters of galaxies A and B. Table 3: N=18 red galaxies.
Ref:	=2001MNRAS.323..688H
by	HAINES C.P. , CLOWES R.G., CAMPUSANO L.E., ADAMSON A.J.
	Mon. Not. R. Astron. Soc., 323, 688-698 (2001)
	The galaxy environment of a quasar at z = 1.226: a possible cluster merger.
o	Fig.5: <[HCC2001] AN> (Nos G1-G4, C1-C3). Fig.6, Table 3: <[HCC2001] Cluster A> (Nos A-B), <[HCC2001] NN> (Nos 1-18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCC2004]
[HCC2004]	(Hu+Cowie+Capak+, 2004)
Write:	<<[HCC2004] NN>>
N:	26
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Subaru 8.3m telescope is used for search for searching Ly-alpha emitter galaxies at z about 5.7. Finding charts in Fig.7.
Ref:	=2004AJ....127..563H
by	HU E.M. , COWIE L.L., CAPAK P., McMAHON R.G., HAYASHINO T., KOMIYAMA Y.
	Astron. J., 127, 563-575 (2004)
	The luminosity function of Lyα emitters at redshift z~5.7.
o	Table 3: <[HCC2004] NN> (Nos 1-26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCC2006]
[HCC2006]	(Hutchings+Cherniawsky+Cutri+, 2006)
Write:	<<[HCC2006] JHHMMSS.ss+DDMMSS.s>>
N:	21
Object:	AGN (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	Optical imaging of 21 low redshift IR-selected AGNs (2MASS AGNs with z<0.3, observable from CFHT). See also [HMC2003].
Ref:	=2006AJ....131..680H
by	HUTCHINGS J.B. , CHERNIAWSKY A., CUTRI R.M., NELSON B.O.
	Astron. J., 131, 680-685 (2006)
	Host galaxies of Two Micron All Sky Survey-selected QSOs at redshift over 0.3.
o	Table 1: <[HCC2006] JHHMMSS.ss+DDMMSS.s> N=21.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCC2011]
[HCC2011]	(Hu+Chen+Chen+, 2011)
Write:	<<[HCC2011] VNN>> <<[HCC2011] SVN>>
N:	42+6
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	Tenagra II 32in telescope observations of N=42 variable stars and N=6 suspected variable stars in the Galactic open cluster NGC 7039.
in source:	NGC 7039
Ref:	=2011PASP..123..671H
by	HU J.-H. , CHEN H.-C., CHEN Y.-T., CHANG D.-C., LIN H.-W., NGEOW C.-C., CHEN W.P., IP W.-H.
	PASP, 123, 671-681 (2011)
	Discovery of variable stars in the field of the Galactic open cluster NGC 7039.
o	Table 2: <[HCC2011] VNN> (Nos V01-V42), <[HCC2011] SVN> (Nos SV1-SV6).
=E=	Catalogue in electronic form as J/PASP/123/671
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCD2001]
[HCD2001]	(Heydari-Maleyari+Charmandaris+Deharveng+, 2001)
Write:	<<[HCD2001] N83B NN>> <<[HCD2001] N11A NN>>
N:	36+18
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of the compact HII region LHA 120-N 83B and the OB association LHA 120-N 11A in the LMC.
in source:	Magellanic Clouds:LMC:LHA 120-N 83B = LHA 120-N 83B
in source:	Magellanic Clouds:LMC:LHA 120-N 11A = LHA 120-N 11A
Ref:	=2001A&A...372..495H
by	HEYDARI-MALAYERI M. , CHARMANDARIS V., DEHARVENG L., ROSA M.R., SCHAERER D., ZINNECKER H.
	Astron. Astrophys., 372, 495-507 (2001)
	HST study of the LMC compact star-forming region N83B.
o	Fig.3: <[HVL90] N83 B-N> (Nos B-2, B-3). Table 3: <[HCD2001] N83B NN> (Nos 1-36).
Ref:	=2001A&A...372..527H
by	HEYDARI-MALAYERI M. , CHARMANDARIS V., DEHARVENG L., ROSA M.R., SCHAERER D., ZINNECKER H.
	Astron. Astrophys., 372, 527-534 (2001)
	HST observations of the LMC compact H II region N11A.
o	Table 2: <[HCD2001] N11A NN> (Nos 1-18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCD2002]
[HCD2002]	(Heydari-Maleyari+Charmandaris+Deharveng+, 2002)
Write:	<<[HCD2002] NNN>>
N:	110
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 study of the region LHA 120-N 160A in the LMC. Finding charts in Figs 2, 3.
in source:	Magellanic Clouds:LMC:LHA 120-N 160A = LHA 120-N 160A
Ref:	=2002A&A...381..941H
by	HEYDARI-MALAYERI M. , CHARMANDARIS V., DEHARVENG L., MEYNADIER F., ROSA M.R., SCHAERER D., ZINNECKER H.
	Astron. Astrophys., 381, 941-950 (2002)
	Resolving the compact HII regions in N160A with HST.
o	A misprint has been detected in the original table : [HCD2002] 46 must correspond to the first line "48" ; the line "46" must correspond to a double.
o	Table 2: <[HCD2002] NNN> (Nos 1-110).
=E=	Catalogue in electronic form as J/A+A/381/941
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCD2009]
[HCD2009]	(Haggard+Cool+Davies, 2009)
Write:	<<[HCD2009] NNNa>>
N:	180+95
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat.	in SIMBAD: Ref. 2009ApJ...697..224H is completely incorporated.
Note:	Chandra ACIS observations of the ome Cen globular cluster. See also CXOHCD. The first character in the source ID represents the radial offset in arcminutes (rounded to the nearest arcminute, except for sources less than 0.5' from the center, which are also assigned a first digit of "1"). The second character (1-4) represents the quadrant in which the source falls (counterclockwise from the northwest quadrant "1"). The last character is a letter (a-l), in the order of azimuthal position (working counterclockwise) within a given annulus and quadrant.
in source:	ome Cen = NGC 5139
Ref:	=2009ApJ...697..224H
by	HAGGARD D. , COOL A.M., DAVIES M.B.
	Astrophys. J., 697, 224-236 (2009)
	A Chandra study of the Galactic globular cluster ω Centauri.
o	Table 1, col(1): <[HCD2009] NNNa> N=180 = Table 1, col(2): <CXOHCD JHHMMSS.ss+DDMMSS.s> N=180.
Ref:	=2018MNRAS.479.2834H
by	HENLEYWILLIS S. , COOL A.M., HAGGARD D., HEINKE C., CALLANAN P., ZHAO Y.
	Mon. Not. R. Astron. Soc., 479, 2834-2852 (2018)
	A Deep X-ray Survey of the globular cluster Omega Centauri.
o	Table 1: <[HCD2009] NNNa> N=95 among (Nos 11d-113b) added.
=E=	Catalogue in electronic form as J/ApJ/697/224
=E=	Catalogue in electronic form as <J/MNRAS/479/2834/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCD99]
[HCD99]	(Heydari-Malayeri+Charmandaris+Deharveng+, 1999)= ([HCD99a])
Write:	<<[HCD99] NN>> <<[HCD99] A>>
N:	79+8
Object:	* (SIMBAD class: Star)
Note:	HST observations of brightest stars towards LHA 115-N 88. (Nos 1-79) in fig., N=63 in Table. Fig.1: (Nos A-H), diffuse HII regions.
in source:	Magellanic Clouds:SMC:LHA 115-N 88 = LHA 115-N 88
Ref:	=1999A&A...347..841H
by	HEYDARI-MALAYERI M. , CHARMANDARIS V., DEHARVENG L., ROSA M.R., ZINNECKER H.
	Astron. Astrophys., 347, 841-849 (1999)
	HST observations of the very young SMC "blob" N88A.
o	Table 1: <[HCD99] NN> N=63 among (Nos 1-79). Fig.1: <[HCD99] A> (Nos A-H).
=E=	Catalogue in electronic form as J/A+A/347/841
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCD99a]
[HCD99a]	(Heydari-Malayeri+Charmandaris+Deharveng+, 1999)
*****	Avoid the usage of [HCD99a], prefer [HCD99]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCD99b]
[HCD99b]	(Hutchings+Crenshaw+Danks+, 1999)
Write:	<<[HCD99b] A>> <<[HCD99b] A'>>
N:	13+2
Object:	Region (SIMBAD class: PartofG = Part of a Galaxy)
Note:	HST STIS and WFPC2 observations of high velocity emission line regions in NGC 4151. See also [HCK98].
in source:	NGC 4151
Ref:	=1999AJ....118.2101H
by	HUTCHINGS J.B. , CRENSHAW D.M., DANKS A.C., GULL T.R., KRAEMER S.B., NELSON C.H., WEISTROP D., KAISER M.E., JOSEPH C.L.
	Astron. J., 118, 2101-2107 (1999)
	High-velocity line emission in the narrow-line region of NGC 4151.
o	Radio knots 1 to 5 in fig. 4 = [CTH90] NGC 4151 C01 to C05.
o	Table2: <[HCD99b] A> (Nos A-J, M-O), <[HCD99b] A'> (Nos D', F').
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HCE
HCE	(Horrobin+Casali+Eiroa)
Origin	of the Acronym: L (1998A&A...330..990G)
Details on Acronym: [HCE2008]
[HCE2008]	(Hora+Cohen+Ellis+, 2008)
Write:	<<[HCE2008] NNN>>
N:	277
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	Spitzer IRAC and MIPS observations of the LMC.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2008AJ....135..726H
by	HORA J.L. , COHEN M., ELLIS R.G., MEIXNER M., BLUM R.D., LATTER W.B., WHITNEY B.A., MEADE M.R., BABLER B.L., INDEBETOUW R., GORDON K., ENGELBRACHT C.W., FOR B.-Q., BLOCK M., MISSELT K., VIJH U., LEITHERER C.
	Astron. J., 135, 726-736 (2008)
	Spitzer SAGE observations of Large Magellanic Cloud planetary nebulae.
o	Table 2: <[HCE2008] NNN> (Nos 1-277).
=E=	Catalogue in electronic form as J/AJ/135/726
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCF2005]
[HCF2005]	(Hatch+Crawford+Fbian+, 2005)
Write:	<<[HCF2005] Region A>> <<[HCF2005] Horseshoe knot>> <<[HCF2005] WWN knot>>
N:	4+1+2
Object:	H-alpha emission region (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	UKIRT spectrographic observations of NGC 1275: detection of rovibrational H2 lines.
in source:	NGC 1275 = 3C 84
Ref:	=2005MNRAS.358..765H
by	HATCH N.A. , CRAWFORD C.S., FABIAN A.C., JOHNSTONE R.M.
	Mon. Not. R. Astron. Soc., 358, 765-773 (2005)
	Detections of molecular hydrogen in the outer filaments of NGC1275.
o	Fig.1, Table 2: <[HCF2005] Region A> (Nos A-D), <[HCF2005] Horseshoe knot> N=1, <[HCF2005] WWN knot> (Nos SW1-SW2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCF2016]
[HCF2016]	(Henshaw+Caselli+Fontani+, 2016) (Not yet in Simbad)
Write:	<<[HCF2016] NN>>
N:	13
Object:	Core (SIMBAD class: denseCore = Dense Core)
Note:	IRAM PdBI 3.2mm dust continuum observations of N=13 cores in the filamentary infrared dark cloud MSXDC G035.39-00.33.
in source:	MSXDC G035.39-0.33
Ref:	=2016MNRAS.463..146H
by	HENSHAW J.D. , CASELLI P., FONTANI F., JIMENEZ-SERRA I., TAN J.C., LONGMORE S.N., PINEDA J.E., PARKER R.J., BARNES A.T.
	Mon. Not. R. Astron. Soc., 463, 146-169 (2016)
	Investigating the structure and fragmentation of a highly filamentary IRDC.
o	Fig. 2, Tables 1-3: <[HCF2016] NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCF97]
[HCF97]	(Hawkins+Clements+Fried+, 1998)
Write:	<<[HCF97] HHMM+DDdA>>
N:	3
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	N=1 gravitational lens candidate, '[HCF97] 2138-431', with 2 quasar images components '[HCF97] 2138-431A' and 'B'
Ref:	=1997MNRAS.291..811H
by	HAWKINS M.R.S. , CLEMENTS D., FRIED J.W., HEAVENS A.F., VERON P., MINTY E.M., VAN DER WERF P.
	Mon. Not. R. Astron. Soc., 291, 811-818 (1997)
	The double quasar Q2138-431: lensing by a dark galaxy?
o	<[HCF97] 2138-431>, <[HCF97] 2138-431A>, <[HCF97] 2138-431B>, N=3
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HCG
HCG	(Hickson, Compact Group)= (H) = (Hick)
Write:	<<HCG NNN>>
N:	100
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	1993ApL....29....1H: atlas of each compact group
Ref:	=1982ApJ...255..382H
by	HICKSON P.
	Astrophys. J., 255, 382-391 (1982)
	Systematic properties of compact groups of galaxies.
o	in ref list:Bautz 1970ApJ.162L.149 instead of 168L.149
o	Table 1: <HCG NNN> (Nos 1-100)
=E=	Catalogue in electronic form as VII/85
=E=	Catalogue in electronic form as VII/213
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HCG
HCG	(Hickson, Compact Group)= (Hick)
Write:	<<HCG NNNa>> <<HCG NNNaN>>
N:	611
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	1993ApL....29....1H: atlas of each compact group. Other galaxies are added to some groups in the literature. The format for galaxies in HCG group is NNNa, but a format NNNaN has been added if the galaxy 'a' in the group 'NNN' have a double nucleus 'a1' and 'a2', or knots. See also [PAM2003] and [PFH2004] for objects 'HCG NNNx' (not galaxies in the group).
Ref:	=1989ApJS...70..687H
by	HICKSON P. , KINDL E., AUMAN J.R.
	Astrophys. J., Suppl. Ser., 70, 687-698 (1989)
	A photometric catalog of compact groups of galaxies.
o	Table 2: <HCG NNNa> N=463 G in HCG NNN groups
Ref:	=1990ApJ...365...86R
by	RUBIN V.C. , HUNTER D.A., FORD W.K.Jr
	Astrophys. J., 365, 86-92 (1990)
	One galaxy from several: the Hickson compact group H 31.
o	<HCG 31a> (Nos 31e, 31f, 31g, 31q) added.
Ref:	=1993AJ....105.1291B
by	BETTONI D. , FASANO G.
	Astron. J., 105, 1291-1307 (1993)
	Morphology of early-type galaxies in compact groups: I.
o	The double nucleus of HCG 74a = [BSR99] HCG 74a n1 and n2 in SIMBAD.
o	<HCG NNNaN> (No. 79b1).
Ref:	=1997ApJ...489L..13I
by	IGLESIAS-PARAMO J. , VILCHEZ J.M.
	Astrophys. J., 489, 13-16 (1997)
	The onset of a three-galaxy merger in the compact group of galaxies HCG 95?
o	<HCG 95c1>, <HCG 95c2>
Ref:	=2004ApJS..153..243L
by	LOPEZ-SANCHEZ A.R. , ESTEBAN C., RODRIGUEZ M.
	Astrophys. J., Suppl. Ser., 153, 243-267 (2004)
	Massive star formation and tidal structures in HCG 31.
o	Table 2:, Fig.1: <HCG 31aN> (Nos a1, f1, f2, h) added.
Ref:	=2005A&A...430..443V
by	VERDES-MONTENEGRO L. , DEL OLMO A., YUN M.S., PEREA J.
	Astron. Astrophys., 430, 443-464 (2005)
	The evolution of HCG 31: Optical and high-resolution HI study.
o	Fig.3, Table 2: <[VDY2005] t-WW> (Nos t-C, t-E, t-S, t-NE, t-NW). Text: <[VDY2005] J0500-0434> N=1. Fig.1, Table 3: <HCG 31aN> (Nos e1-e5, f3-f7, g1-g8).
Ref:	=2006AJ....132..570M
by	MENDES DE OLIVEIRA C.L. , TEMPORIN S., CYPRIANO E.S., PLANA H., AMRAM P., SODRE L.Jr, BALKOWSKI C.
	Astron. J., 132, 570-581 (2006)
	The K luminosity-metallicity relation for dwarf galaxies and the tidal dwarf galaxies in the tails of HCG 31.
o	Table 2: <HCG 31aN> (Nos h1-h2, r, r1) added.
=E=	Catalogue in electronic form as VII/213
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HCG2000]
[HCG2000]	(Holzapfel+Carlstrom+Greco+, 2000)= (BDF)
Write:	<<[HCG2000] BDFN JHHMMSS.s+DDMMSS>>
N:	5
Object:	(Ras) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=5 point sources in BDF (BIMA Deep Field) (BIMA = Berkeley-Illinois-Maryland Assoc.). See also [DHC2002].
Ref:	=2000ApJ...539...57H
by	HOLZAPFEL W.L. , CARLSTROM J.E., GREGO L., HOLDER G., JOY M., REESE E.D.
	Astrophys. J., 539, 57-66 (2000)
	Limits on arcminute-scale cosmic microwave background anisotropy at 28.5 GHz.
o	Table 2: <[HCG2000] BDFN JHHMMSS.s+DDMMSS> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCG2001]
[HCG2001]	(Harris+Calzetti+Gallagher+, 2001)
Write:	<<[HCG2001] Cl* NN>> <<[HCG2001] Obj NNN>>
N:	45+330
Object:	Cluster of * + *inCl (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of M 83. N=45 clusters of stars, and N=330 fainter objects (star clusters or individual stars) detected as part of the diffuse stellar population of M 83.
in source:	M 83 = NGC 5236
Ref:	=2001AJ....122.3046H
by	HARRIS J. , CALZETTI D., GALLAGHER III J.S., CONSELICE C.J., SMITH D.A.
	Astron. J., 122, 3046-3064 (2001)
	Young clusters in the nuclear starburst of M83.
o	Table 2: <[HCG2001] Cl* NN> (Nos 1-45). Table 3: <[HCG2001] Obj NNN> (Nos 1-330).
=E=	Catalogue in electronic form as J/AJ/122/3046
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCG2004]
[HCG2004]	(Harris+Calzetti+Gallagher+, 2004)
Write:	<<[HCG2004] NGC 3077 C NN>> <<[HCG2004] NGC 5253 C NN>> <<[HCG2004] NGC 3077 NC NNN>> <<[HCG2004] NGC 5253 NC NNN>>
N:	55+33+243+391
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of NGC 3077 and NGC 5253. Search for clusters of stars (letter C in the format), and other objects (letters NC for Non Cluster in the format).
in source:	NGC 3077
in source:	NGC 5253
Ref:	=2004ApJ...603..503H
by	HARRIS J. , CALZETTI D., GALLAGHER III J.S., SMITH D.A., CONSELICE C.J.
	Astrophys. J., 603, 503-522 (2004)
	The recent cluster formation histories of NGC 5253 and NGC 3077: environmental impact on star formation.
o	Table 3: <[HCG2004] NGC 3077 C NN> (Nos 1-55). Table 4: <[HCG2004] NGC 5253 C NN> (Nos 1-33). Table 5: <[HCG2004] NGC 3077 NC NNN> (Nos 1-243). Table 6: <[HCG2004] NGC 5253 NC NNN> (Nos 1-391).
=E=	Catalogue in electronic form as J/ApJ/603/503
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCG98]
[HCG98]	(Heithausen+Corneliussen+Grossmann, 1998) (Not yet in Simbad)
Write:	<<[HCG98] NN>>
N:	17
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
in source:	NAME MCLD 126.6+24.5
Ref:	=1998A&A...330..311H
by	HEITHAUSEN A. , CORNELIUSSEN U., GROSSMANN V.
	Astron. Astrophys., 330, 311-320 (1998)
	The SO-to-CS abundance ratio in molecular cirrus clouds.
o	Table 2: Clouds LLL.l+BB.b are 'HSVMT NN'
o	Table 3: <[HCG98] NN> (Nos 1-17)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HCH
HCH	(Holland+Cote+Hesser)
*****	Avoid the usage of HCH, prefer [HCH99]
Origin	of the Acronym: L (2004ApJS..150..367P)
Details on Acronym: [HCH93]
[HCH93]	(Hatzidimitriou+Cannon+Hawkins, 1993)
Write:	<<[HCH93] NN>>
N:	54
Object:	* (SIMBAD class: Star)
Note:	N=54 * among (Nos 1-63)
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1993MNRAS.261..873H
by	HATZIDIMITRIOU D. , CANNON R.D., HAWKINS M.R.S.
	Mon. Not. R. Astron. Soc., 261, 873-882 (1993)
	Kinematics in the outer parts of the SMC.
o	Table 1: <[HCH93] NN> N=54 among (Nos 1-63).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCH99]
[HCH99]	(Holland+Cote+Hesser, 1999)= (HCH)
Write:	<<[HCH99] NNN>>
N:	21+61
Object:	GlCl + ? (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of NGC 5128. Table 2: (Nos 1-21), GCl candidates. Table 3: (Nos 101-161), Extended objects. Finding charts of GCl.
in source:	Cen A = NGC 5128
Ref:	=1999A&A...348..418H
by	HOLLAND S. , COTE P., HESSER J.E.
	Astron. Astrophys., 348, 418-436 (1999)
	Globular clusters in NGC 5128.
o	In introduction, globular cluster C44 is [VHH81] 44.
o	Table 2: <[HCH99] NN> (Nos 1-21). Table 3: <[HCH99] NNN> (Nos 101-161).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCJ2009]
[HCJ2009]	(Hicken+Challis+Jha+, 2009)
Write:	<<[HCJ2009] SN YYYYA NN>> <<[HCJ2009] SN YYYYaa NN>>
N:	2481
Object:	Comparison * (SIMBAD class: Star)
Note:	FLWO 1.2m telescope observations of comparison stars near 185 type Ia supernovae.
Ref:	=2009ApJ...700..331H
by	HICKEN M. , CHALLIS P., JHA S., KIRSHNER R.P., MATHESON T., MODJAZ M., REST A., WOOD-VASEY W.M., BAKOS G., BARTON E.J., BERLIND P., BRAGG A., BRICENO C., BROWN W.R., CALDWELL N., CALKINS M., CHO R., CIUPIK L., CONTRERAS M., DENDY K.-C., DOSAJ A., DURHAM N., ERIKSEN K., ESQUERDO G., EVERETT M., FALCO E., FERNANDEZ J., GABA A., GARNAVICH P., GRAVES G., GREEN P., GRONER T., HERGENROTHER C., HOLMAN M.J., HRADECKY V., HUCHRA J., HUTCHISON B., JERIUS D., JORDAN A., KILGARD R., KRAUSS M., LUHMAN K., MACRI L., MARRONE D., McDOWELL J., McINTOSH D., McNAMARA B., MEGEATH T., MOCHEJSKA B., MUNOZ D., MUZEROLLE J., NARANJO O., NARAYAN G., PAHRE M., PETERS W., PETERSON D., RINES K., RIPMAN B., ROUSSANOVA A., SCHILD R., SICILIA-AGUILAR A., SOKOLOSKI J., SMALLEY K., SMITH A., SPAHR T., STANEK K.Z., BARMBY P., BLONDIN S., STUBBS C.W., SZENTGYORGYI A., TORRES M.A.P., VAZ A., VIKHLININ A., WANG Z., WESTOVER M., WOODS D., ZHAO P.
	Astrophys. J., 700, 331-357 (2009)
	CfA3: 185 type Ia supernova light curves from the CfA.
o	Tables 3-4: <[HCJ2009] SN YYYYA NN>, <[HCJ2009] SN YYYYaa NN> N=2481.
=E=	Catalogue in electronic form as <J/ApJ/700/331/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCJ97]
[HCJ97]	(Hakala+Charles+Johnston+, 1997)
Write:	<<[HCJ97] NN>>
N:	10
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT HRI observations.
in source:	NGC 5904 = M 5
Ref:	=1997MNRAS.285..693H
by	HAKALA P.J. , CHARLES P.A., JOHNSTON H.M., VERBUNT F.
	Mon. Not. R. Astron. Soc., 285, 693-695 (1997)
	X-ray detection of the dwarf nova V101 in M5.
o	Table 1: <[HCJ97] N> (Nos 1-5)
Ref:	=2001A&A...368..137V
by	VERBUNT F.
	Astron. Astrophys., 368, 137-159 (2001)
	A census with ROSAT of low-luminosity X-ray sources in globular clusters.
o	Table 2: see also [FLM96], [HCJ97], [HG83b], [HGB93], [JVH94], [JVH96], [RDL94].
o	Table 2: <[V2001] NGC NNNN XNNa> N=49, <[V2001] JHHMMSS.ss+DDMMSS.s> N=2, <[FLM96] M 13 Aa> (Nos F, Ga-Gb, R-T) added, <[HCJ97] NN> (Nos 6-10) added, <[HGB93] A> (No. G) added, <[JVH94] NGC 6626 NNa> (Nos 5-12, 2a-2c) added, <[JVH94] NGC 6656 N> (No. 9) added, <[JVH94] NGC 7099 NN> (No. 13) added, <[JVH96] NGC 6121 NN> (Nos 7-10) added, <[JVH96] NGC 6352 NN> (No. 17) added, <[JVH96] NGC 6366 NN> (Nos 7-8) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCK2007]
[HCK2007]	(Hardcastle+Croston+Kraft, 2007) (Not yet in Simbad)
Write:	<<[HCK2007] 3C NNN W>> <<[HCK2007] 3C NNN.N W>> <<[HCK2007] 3C NNN WXN>> <<[HCK2007] 3C NNN.N WXN>>
N:	7+5
Object:	Lobe + (X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of four radio galaxies.
in source:	3C 227
in source:	3C 327
in source:	3C 390.3
in source:	3C 403
Ref:	=2007ApJ...669..893H
by	HARDCASTLE M.J. , CROSTON J.H., KRAFT R.P.
	Astrophys. J., 669, 893-904 (2007)
	A Chandra study of particle acceleration in the multiple hot spots of nearby radio galaxies.
o	Table 4, col(2): <[HCK2007] 3C NNN W>, <[HCK2007] 3C NNN.N W>, N=7. Table 4, col(3): <[HCK2007] 3C NNN WXN>, <[HCK2007] 3C NNN.N WXN>, N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCK2012]
[HCK2012]	(Hicken+Challis+Kirshner+, 2012) (Not yet in Simbad)
Write:	<<[HCK2012] JHHMMSS.sss+DDMMSS.ss>>
N:	2301
Object:	* (SIMBAD class: Star)
Note:	N=2301 comparison stars in the field of N=94 SNe.
Ref:	=2012ApJS..200...12H
by	HICKEN M. , CHALLIS P., KIRSHNER R.P., REST A., CRAMER C.E., WOOD-VASEY W.M., BAKOS G., BERLIND P., BROWN W.R., CALDWELL N., CALKINS M., CURRIE T., DE KLEER K., ESQUERDO G., EVERETT M., FALCO E., FERNANDEZ J., FRIEDMAN A.S., GRONER T., HARTMAN J., HOLMAN M.J., HUTCHINS R., KEYS S., KIPPING D., LATHAM D., MARION G.H., NARAYAN G., PAHRE M., PAL A., PETERS W., PERUMPILLY G., RIPMAN B., SIPOCZ B., SZENTGYORGYI A., TANG S., TORRES M.A.P., VAZ A., WOLK S., ZEZAS A.
	Astrophys. J., Suppl. Ser., 200, 12 (2012)
	CfA4: light curves for 94 type Ia supernovae.
o	Table 4: <[HCK2012] JHHMMSS.sss+DDMMSS.ss> N=2301.
=E=	Catalogue in electronic form as J/ApJS/200/12
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCK98]
[HCK98]	(Hutchings+Crenshaw+Kaiser+, 1998)
Write:	<<[HCK98] NNa>>
N:	54
Object:	Cloud (SIMBAD class: Cloud)
Note:	HST STIS observations of the nuclear region of NGC 4151. Map in Fig.3 (1st ref.) and Figs 4, 5 (2nd ref.). See also [HCD99b].
in source:	NGC 4151
Ref:	=1998ApJ...492L.115H
by	HUTCHINGS J.B. , CRENSHAW D.M., KAISER M.E., KRAEMER S.B., WEISTROP D., BAUM S., BOWERS C.W., FEINBERG L.D., GREEN R.F., GULL T.R., HARTIG G.F., HILL G., LINDLER D.J.
	Astrophys. J., 492, 115-120 (1998)
	Gas cloud kinematics near the nucleus of NGC 4151.
o	Table 1, Fig.3: <[HCK98] NNa> (Nos 1-42, 16a)
Ref:	=2000ApJ...528..260K
by	KAISER M.E. , BRADLEY II L.D., HUTCHINGS J.B., CRENSHAW D.M., GULL T.R., KRAEMER S.B., NELSON C.H., RUIZ J., WEISTROP D.
	Astrophys. J., 528, 260-275 (2000)
	The resolved narrow-line region in NGC 4151.
o	T.3: Clouds 'a' = '[HCD99b] A'
o	Table 2: <[HCK98] NNa> (Nos 19a, 21x, 44-51) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HCl
HCl	(Heiles Cloud)= (HC) = (Heiles)
Write:	<<HCl N>> <<HCl NA>> <<HCl NAN>>
N:	23
Object:	Cloud + Part of Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Ref:	=1968ApJ...151..919H
by	HEILES C.
	Astrophys. J., 151, 919-934 (1968)
	Normal OH emission and interstellar clouds.
o	Tables 2, 3, Fig.: <HCL N> (Nos 1-2, 4-5), <HCL NA> N=14
Ref:	=1984A&A...138..371C
by	CERNICHARO J. , GUELIN M., ASKNE J.
	Astron. Astrophys., 138, 371-379 (1984)
	TMC 1-like cloudlets in HCL 2.
o	<HCL 2A>, Nos 2A, 2B, 2C
Ref:	=1988ApJ...324..311H
by	HEYER M.H.
	Astrophys. J., 324, 311-320 (1988)
	The magnetic evolution of the Taurus molecular clouds. II. A reduced role of the magnetic field in dense core regions.
o	(Erratum) + erratum vol. 329, 1039
o	Table 2: <HCl 2A> (Nos 2A-2F), <HCl 2GN> Nos 2G1, 2G2, <Barnard NNNA> (Nos 217A-217G) and (Nos 18A-18I)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HCL2018]
[HCL2018]	(Harris+Cox+Looney+, 2018)
Write:	<<[HCL2018] VLA 1623Aa>>
N:	2
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 7 observations of N=2 components of [LMW2000] VLA 1623A.
in source:	[LMW2000] VLA 1623A
Ref:	=2018ApJ...861...91H
by	HARRIS R.J. , COX E.G., LOONEY L.W., LI Z.-Y., YANG H., FERNANDEZ-LOPEZ M., KWON W., SADAVOY S., SEGURA-COX D., STEPHENS I., TOBIN J.
	Astrophys. J., 861, 91-91 (2018)
	ALMA observations of polarized 872 µm dust emission from the protostellar systems VLA 1623 and L1527.
o	Fig. 3, Table 2: <[HCL2018] VLA 1623Aa> (Nos VLA 1623Aa-VLA 1623Ab).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HCM
HCM	(Hu+Cowie+McMahon+)
*****	Avoid the usage of HCM, prefer [HCM2002]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HCM
HCM	(Hu+Cowie+McMahon)
*****	Avoid the usage of HCM, prefer [HMC99b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HCM2000]
[HCM2000]	(Hurley+Cline+Mazets+, 2000)= (VLA) (Not yet in Simbad)
Write:	<<[HCM2000] VLA N>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=2000ApJ...534L..23H
by	HURLEY K. , CLINE T., MAZETS E., APTEKAR R., GOLENETSKII S., FREDERIKS D., FRAIL D., KULKARNI S., TROMBKA J., McCLANAHAN T., STARR R., GOLDSTEN J.
	Astrophys. J., 534, 23-25 (2000)
	Interplanetary network localization of GRB 991208 and the discovery of its afterglow.
o	Fig.3: <[HCM2000] VLA N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCM2002]
[HCM2002]	(Hu+Cowie+McMahon+, 2002)= (HCM)
Write:	<<[HCM2002] 6A>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck and Subaru observations.
Ref:	=2002ApJ...568L..75H
by	HU E.M. , COWIE L.L., McMAHON R.G., CAPAK P., IWAMURO F., KNEIB J.-P., MAIHARA T., MOTOHARA K.
	Astrophys. J., 568, 75-79 (2002)
	A redshift z=6.56 galaxy behind the cluster Abell 370.
o	(Erratum) erratum vol. 576, p. L99 (2002)
o	Object BO 39 in fig.1 is BOW ACO 370 CC039
o	<[HCM2002] 6A> N=1 = <NAME HCM 6A>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCM87]
[HCM87]	(Hecquet+Coupinot+Maucherat, 1987)
Write:	<<[HCM87] NN>>
N:	44
Object:	Clump (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Observations of Mrk 297 at the 2m telescope of Pic-du-Midi Observatory.
in source:	Mrk 297
Ref:	=1987A&A...183...13H
by	HECQUET J. , COUPINOT G., MAUCHERAT A.J.
	Astron. Astrophys., 183, 13-15 (1987)
	Markarian 297 knots.
o	in ref list KEEL 1978AJ.....83....1K instead of ApJ.83
o	Table 1: <[HCM87] NN> (Nos 1-44).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCM97]
[HCM97]	(Hatzidimitriou+Croke+Morgan+, 1997)
Write:	<<[HCM97] NN>>
N:	16
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Note:	See also [MH95] for C*
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1997A&AS..122..507H
by	HATZIDIMITRIOU D. , CROKE B.F., MORGAN D.H., CANNON R.D.
	Astron. Astrophys., Suppl. Ser., 122, 507-513 (1997)
	Kinematics of carbon stars in the outer regions of the Small Magellanic Cloud.
o	Table 1b: <[HCM97] NN> (Nos 1-16)
=E=	Catalogue in electronic form as J/A+AS/122/507
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCM99]
[HCM99]	(Hutchings+Crampton+Morris+, 1999) (Not yet in Simbad)
Write:	<<[HCM99] HHMM+DDd NN>> <<[HCM99] HHMM+DDd Host>> <<[HCM99] HHMM+DDd Wisp>> <<[HCM99] HHMM+DDd Knot>>
N:	51
Object:	* + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	* and G in the field of 8 QSOs.
Ref:	=1999AJ....117.1109H
by	HUTCHINGS J.B. , CRAMPTON D., MORRIS S.L., DURAND D., STEINBRING E.
	Astron. J., 117, 1109-1121 (1999)
	QSO hosts and environments at z=0.9-4.2: JHK images with adaptive optics.
o	p. 1115, QSO 1345+580 = 1345+584.
o	Tables 3-10: <[HCM99] HHMM+DDd NN>, <[HCM99] HHMM+DDd Host>, <[HCM99] HHMM+DDd Wisp>, <[HCM99] HHMM+DDd Knot>, N=51.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HCNOP
HCNOP	(HCN, Outflow Peak) (Not yet in Simbad)
Write:	<<HCNOP NN>>
N:	10
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Note:	See also [C2005b]
in source:	NGC 1333:[JCC87] IRAS 4 = [JCC87] IRAS 4
Ref:	=2001ApJ...553..219C
by	CHOI M.
	Astrophys. J., 553, 219-226 (2001)
	High-resolution observations of the molecular clouds in the NGC 1333 IRAS 4 region.
o	Fig.1: <HCNOP N> (Nos 1-9).
Ref:	=2005ApJ...630..976C
by	CHOI M.
	Astrophys. J., 630, 976-986 (2005)
	Variability of the NGC 1333 IRAS 4A outflow: silicon monoxide observations.
o	Table 1, Fig.2: <SiOOP NNa> (Nos 1a, 1b, 2-17). Fig.4a: <HCNOP NN> (No. 10) added.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HCO2007]
[HCO2007]	(Hofner+Cesaroni+Olmi+, 2007)
Write:	<<[HCO2007] WN>> <<[HCO2007] I20var>>
N:	3+1
Object:	(cm) (SIMBAD class: cmRad = Centimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 3.6cm continuum emission in IRAS 20126+4104.
in source:	IRAS 20126+4104
Ref:	=2007A&A...465..197H
by	HOFNER P. , CESARONI R., OLMI L., RODRIGUEZ L.F., MARTI J., ARAYA E.
	Astron. Astrophys., 465, 197-205 (2007)
	Sub-arcsecond resolution radio continuum observations of IRAS 20126+4104.
o	Fig.1, Table 1: <[HCO2007] WN> (Nos N1, N2, S). Paragr. 3.2: <[HCO2007] I20var> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCP2005]
[HCP2005]	(Hamaguchi+Corcoran+Petre+, 2005)
Write:	<<[HCP2005] XW>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton and Chandra observations of R CrA star-forming core.
in source:	NAME R CrA Cloud
Ref:	=2005ApJ...623..291H
by	HAMAGUCHI K. , CORCORAN M.F., PETRE R., WHITE N.E., STELZER B., NEDACHI K., KOBAYASHI N., TOKUNAGA A.T.
	Astrophys. J., 623, 291-301 (2005)
	Discovery of extremely embedded X-ray sources in the R Coronae Australis star-forming core.
o	Table 2: <[HCP2005] XW> (Nos XE, XW).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCP2006]
[HCP2006]	(Harvey+Chapman+Lai+, 2006)= (Spitzer)
Write:	<<[HCP2006] Cluster A>> <<[HCP2006] Cluster B NN>>
N:	2+24
Object:	Cluster of * + *inCl (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Spitzer Space Telescope IRAC observations of the Serpens cloud.
in source:	NAME Serpens Cloud
Ref:	=2006ApJ...644..307H
by	HARVEY P.M. , CHAPMAN N., LAI S.-P., EVANS II N.J., ALLEN L.E., JORGENSEN J.K., MUNDY L.G., HUARD T.L., PORRAS A., CIEZA L., MYERS P.C., MERIN B., VAN DISHOECK E.F., YOUNG K.E., SPIESMAN W., BLAKE G.A., KOERNER D.W., PADGETT D.L., SARGENT A.I., STAPELFELDT K.R.
	Astrophys. J., 644, 307-325 (2006)
	The Spitzer c2d survey of large, nearby, insterstellar clouds. II. Serpens observed with IRAC.
o	Paragr.7: Ser/G3-G6 = CoKu Ser G3 to CoKu Ser G6.
o	Text: <[HCP2006] Cluster A> (Nos A-B). Table 4: <[HCP2006] Cluster B NN> (Nos 1-24).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCP2011]
[HCP2011]	(Hempel+Cristobal-Hornillos+Prieto+, 2011)
Write:	<<[HCP2011] ero JHHMMSS.ss+DDMMSS.s>>
N:	102
Object:	Extremely Red G (SIMBAD class: Galaxy)
Note:	N=102 extremely red galaxies with F814W-Ks≥4 found within the Galaxy Origins and Young Assembly (GOYA) survey.
in source:	NAME Groth-Westphal Strip
Ref:	=2011MNRAS.414.2246H
by	HEMPEL A. , CRISTOBAL-HORNILLOS D., PRIETO M., TRUJILLO I., BALCELLS M., LOPEZ-SANJUAN C., ABREU D., ELICHE-MORAL M.C., DOMINGUEZ-PALMERO L.
	Mon. Not. R. Astron. Soc., 414, 2246-2264 (2011)
	The morphologies and masses of extremely red galaxies in the Groth Strip.
o	Tables A1-A2: <[HCP2011] ero JHHMMSS.ss+DDMMSS.s> N=108.
=E=	Catalogue in electronic form as <J/MNRAS/414/2246/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCP84]
[HCP84]	(He+Cannon+Peacock+, 1984)= (U)
Write:	<<[HCP84] NN>> <<[HCP84] UNN>>
N:	53+29
Object:	Poss. QSO + (UV) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 2: (Nos 1-53), emission-line QSO candidates. Table 3: (Nos U1-U29), UV excess candidates. Identif. charts
Ref:	=1984MNRAS.211..443H
by	HE X.-T. , CANNON R.D., PEACOCK J.A., SMITH M.G., OKE J.B.
	Mon. Not. R. Astron. Soc., 211, 443-459 (1984)
	A search for quasars in the Virgo cluster region.
o	Table 2: <[HCP84] NN> (Nos 1-53). Table 3: <[HCP84] UNN> (Nos U1-U29)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCP92]
[HCP92]	(Henning+Chini+Pfau, 1992)
Write:	<<[HCP92] Clump N>>
N:	7
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
in source:	NAME Mon R2 GMC
Ref:	=1992A&A...263..285H
by	HENNING T. , CHINI R., PFAU W.
	Astron. Astrophys., 263, 285-291 (1992)
	Submm/mm observations of the Monoceros R2 cloud core.
o	Table 1: <[HCP92] Clump N> (Nos 1-7)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCR2001]
[HCR2001]	(Held+Clementini+Rizzi+, 2001) (Not yet in Simbad)
Write:	<<[HCR2001] VNNNNNN>>
N:	7
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
in source:	UGC 5470 = Leo I
Ref:	=2001ApJ...562L..39H
by	HELD E.V. , CLEMENTINI G., RIZZI L., MOMANY Y., SAVIANE I., DI FABRIZIO L.
	Astrophys. J., 562, 39-42 (2001)
	RR Lyrae variable stars in the dwarf spheroidal galaxy Leo I.
o	Figs 1, 3: <[HCR2001] VNNNNNN> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HCS
HCS	(Heyer+Carpenter+Snell)
*****	Avoid the usage of HCS, prefer [HCS2001]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HCS2000]
[HCS2000]	(Hopkins+Connolly+Szalay, 2000)= (NIC)
Write:	<<[HCS2000] NIC JHHMMSS.ss+DDMMSS.s>>
N:	38
Object:	G (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST NICMOS observations. N=38 galaxies with possible H-alpha emission.
Ref:	=2000AJ....120.2843H
by	HOPKINS A.M. , CONNOLLY A.J., SZALAY A.S.
	Astron. J., 120, 2843-2850 (2000)
	Star formation in galaxies between redshifts of 0.7 and 1.8.
o	able 1: <[HCS2000] NIC JHHMMSS.ss+DDMMSS.s> N=38.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCS2001]
[HCS2001]	(Heyer+Carpenter+Snell)
Write:	<<[HCS2001] NNNNN>>
N:	10156
Object:	Cloud (SIMBAD class: MolCld = Molecular Cloud)
Note:	FCRAO CO survey: study of molecular regions in the Outer Galaxy. The identified objects includes both small, isolated clouds and clumps within larger cloud complexes.
Ref:	=2001ApJ...551..852H
by	HEYER M.H. , CARPENTER J.M., SNELL R.L.
	Astrophys. J., 551, 852-866 (2001)
	The equilibrium state of molecular regions in the outer Galaxy.
o	Catalog: <[HCS2001] NNNNN> (Nos 1-10156).
=E=	Catalogue in electronic form as J/ApJ/551/852
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCS2005]
[HCS2005]	(Hadfield+Crowther+Schild+, 2005)
Write:	<<[HCS2005] NNN>>
N:	221
Object:	WR* (SIMBAD class: WolfRayet* = Wolf-Rayet)
Note:	VLT FORS2 observations. Catalogue Wolf-Rayet stars in M 83: (Nos 1-132) are confirmed WR sources, (Nos 133-221) are not confirmed.
in source:	M 83 = NGC 5236
Ref:	=2005A&A...439..265H
by	HADFIELD L.J. , CROWTHER P.A., SCHILD H., SCHMUTZ W.
	Astron. Astrophys., 439, 265-277 (2005)
	A spectroscopic search for the non-nuclear Wolf-Rayet population of the metal-rich spiral galaxy M83.
o	Tables A1, A2: <[HCS2005] NNN> (Nos 1-221).
=E=	Catalogue in electronic form as J/A+A/439/265
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCS2007]
[HCS2007]	(Hilton+Collins+Stanford+, 2007)
Write:	<<[HCS2007] NN>>
N:	27
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Keck DEIMOS and VLT FORS2 observations of ClG J2215-1738.
in source:	ClG J2215-1738
Ref:	=2007ApJ...670.1000H
by	HILTON M. , COLLINS C.A., STANFORD S.A., LIDMAN C., DAWSON K.S., DAVIDSON M., KAY S.T., LIDDLE A.R., MANN R.G., MILLER C.J., NICHOL R.C., ROMER A.K., SABIRLI K., VIANA P.T.P., WEST M.J.
	Astrophys. J., 670, 1000-1009 (2007)
	The XMM cluster survey: the dynamical state of XMMXCS J2215.9-1738 at z = 1.457.
o	Table 2: <[HCS2007] NN> (Nos 1-27).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCS2018]
[HCS2018]	(Hasinger+Capak+Salvato+, 2018)= ([HCS2018a])
Write:	<<[HCS2018] JDDD.dddd+DD.dddd>>
N:	10728
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Keck II DEIMOS spectroscopy of N=10728 objects in the COSMOS field.
in source:	NAME COSMOS Field
Ref:	=2018ApJ...858...77H
by	HASINGER G. , CAPAK P., SALVATO M., BARGER A.J., COWIE L.L., FAISST A., HEMMATI S., KAKAZU Y., KARTALTEPE J., MASTERS D., MOBASHER B., NAYYERI H., SANDERS D., SCOVILLE N.Z., SUH H., STEINHARDT C., YANG F.
	Astrophys. J., 858, 77-77 (2018)
	The DEIMOS 10k spectroscopic survey catalog of the COSMOS field.
o	Table 3: <[HCS2018] JDDD.dddd+DD.dddd> N=10728.
=E=	Catalogue in electronic form as <J/ApJ/858/77/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCS2018a]
[HCS2018a]	(Hasinger+Capak+Salvato+, 2018)
*****	Avoid the usage of [HCS2018a], prefer [HCS2018]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCS2018b]
[HCS2018b]	(Hill+Chapman+Scott+, 2018)
Write:	<<[HCS2018b] UDSNN>> <<[HCS2018b] SSA22-NN>> <<[HCS2018b] COSMOSNNa>> <<[HCS2018b] LHNNNa>> <<[HCS2018b] EGSNN>>
N:	23+8+15+20+11
Object:	smm G (SIMBAD class: Galaxy)
Note:	SMA 860µm observations of N=23+8+15+20+11 galaxies in five of the seven S2CLS fields (UKIDSS UDS, SSA 22, COSMOS, Lockman Hole North LHN, and Extended Groth Strip EGS, respectively).
in source:	SSA 22
in source:	NAME COSMOS Field
in source:	NAME Lockman Hole
in source:	NAME Extended Groth Strip
Ref:	=2018MNRAS.477.2042H
by	HILL R. , CHAPMAN S.C., SCOTT D., PETITPAS G., SMAIL I., CHAPIN E.L., GURWELL M.A., PERRY R., BLAIN A.W., BREMER M.N., CHEN C.-C., DUNLOP J.S., FARRAH D., FAZIO G.G., GEACH J.E., HOWSON P., IVISON R.J., LACAILLE K., MICHALOWSKI M.J., SIMPSON J.M., SWINBANK A.M., VAN DER WERF P.P., WILNER D.J.
	Mon. Not. R. Astron. Soc., 477, 2042-2067 (2018)
	High-resolution SMA imaging of bright submillimetre sources from the SCUBA-2 Cosmology Legacy Survey.
o	Table A1: <[HCS2018b] UDSNN> N=23 among (Nos UDS03-UDS40). Table A2: <[HCS2018b] SSA22-NN> N=8 among (Nos SSA22-02 to SSA22-09). Table A3: <[HCS2018b] COSMOSNNa> N=15 among (Nos COSMOS01-COSMOS25). Table A4: <[HCS2018b] LHNNNa> (Nos LHN01-LHN02, LHN03a-LHN03b, LHN04-LHN12, LHN13a-LHN13b, LHN14-LHN18). Table A5: <[HCS2018b] EGSNN> (Nos EGS01-EGS11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCS2020]
[HCS2020]	(Hill+Chapman+Scott+, 2020)
Write:	<<[HCS2020] SPIREa>> <<[HCS2020] CNN>> <<[HCS2020] NN>> <<[HCS2020] SPIREcN>> <<[HCS2020] NLN>>
N:	5+32
Object:	(smm) + G (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	N=5 red Herschel sources, ‘red’ defined as S500μm >S350μm >S250μm, using Herschel SPIRE data (format SPIREa). ALMA observations of N=32 galaxies in the the protocluster SPT-CL J2349-5638. The galaxies are named according to the region where they are located, where ‘C’ refers to the core (N=23), ‘N’ refers to the northern component (N=3), and ‘SPIREc’ refers to the red Herschel source SPIREc (N=3). Continuum-only sources are designated as ‘NL (no line).
in source:	SPT-CL J2349-5638
Ref:	=2020MNRAS.495.3124H
by	HILL R. , CHAPMAN S., SCOTT D., APOSTOLOVSKI Y., ARAVENA M., BETHERMIN M., BRADFORD C.M., CANNING R.E.A., DE BREUCK C., DONG C., GONZALEZ A., GREVE T.R., HAYWARD C.C., HEZAVEH Y., LITKE K., MALKAN M., MARRONE D.P., PHADKE K., REUTER C., ROTERMUND K., SPILKER J., VIEIRA J.D., WEISS A.
	Mon. Not. R. Astron. Soc., 495, 3124-3159 (2020)
	Megaparsec-scale structure around the protocluster core SPT2349-56 at z = 4.3.
o	Fig. 1: <[HCS2020] SPIREa> (Nos SPIREa-SPIREe). Fig. 2, Tables 2-3: <[HCS2020] CNN> (Nos C1-C23), <[HCS2020] NN> (Nos N1-N3), <[HCS2020] NLN> (Nos NL1-NL3), <[HCS2020] SPIREcN> (Nos SPIREc1-SPIREc3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCS79]
[HCS79]	(Haynes+Caswell+Simons, 1979)
Write:	<<[HCS79] BHHMMSS.s+DDMMSS.s>>
N:	915
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Detection of 915 sources at 5GHz in the Galactic Plane with the Parkes radiotelescope.
Ref:	=1979AuJPA..48....1H
by	HAYNES R.F. , CASWELL J.L., SIMONS L.W.J.
	Australian J. Phys. Astrophys. Suppl., 48, 1-30 (1979)
	A catalogue of 5 GHz Galactic Plane Sources.
o	Catalogue: <[HCS79] BHHMMSS.s+DDMMSS.s> N=915.
=E=	Catalogue in electronic form as VIII/20
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCT2009]
[HCT2009]	(Hui+Cheng+Taam, 2009) (Not yet in Simbad)
Write:	<<[HCT2009] M28A>>
N:	8
Object:	Millisecond pulsar (SIMBAD class: Pulsar)
Note:	Chandra ACIS observation of N=8 millisecond pulsars in M 28.
in source:	M 28 = NGC 6626
Ref:	=2009ApJ...700.1233H
by	HUI C.Y. , CHENG K.S., TAAM R.E.
	Astrophys. J., 700, 1233-1241 (2009)
	Diffuse X-ray emission in globular cluster cores.
o	Fig. 1: <[HCT2009] M28A> N=8 among (Nos A-J).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCV2005]
[HCV2005]	(Hannikainen+Charles+Van Zyl+, 2005)
Write:	<<[HCV2005] A>>
N:	4
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra HRC observations of faint X-ray sources in M 15.
in source:	M 15 = NGC 7078
Ref:	=2005MNRAS.357..325H
by	HANNIKAINEN D.C. , CHARLES P.A., VAN ZYL L., KONG A.K.H., HOMER L., HAKALA P., NAYLOR T., DAVIES M.B.
	Mon. Not. R. Astron. Soc., 357, 325-332 (2005)
	The X-ray source population of the globular cluster M15: Chandra high-resolution imaging.
o	The planetary nebula K648 = PN Ku 648
o	Table 3: <[HCV2005] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HCW
HCW	(Hu+Cowie+Wang)
Write:	<<HCW ACO NNNN N>>
N:	44
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=44 G in 14 ACO ClG.
in source:	ACO 85
in source:	ACO 133
in source:	ACO 262
in source:	ACO 401
in source:	ACO 496
in source:	ACO 644
in source:	ACO 754
in source:	ACO 978
in source:	ACO 1126
in source:	ACO 1775
in source:	ACO 2029
in source:	ACO 2052
in source:	ACO 2142
Ref:	=1985ApJS...59..447H
by	HU E.M. , COWIE L.L., WANG Z.-H.
	Astrophys. J., Suppl. Ser., 59, 447-498 (1985)
	Long-slit spectroscopy of gas in the cores of X-ray luminous clusters.
o	Table 2: <HCW ACO 85 N> (Nos 1-7), <HCW ACO 133 N> (Nos 1-2), <HCW ACO 262 N> (No. 1), <HCW ACO 401 N> (No. 1), <HCW ACO 496 N> (Nos 1-3), <HCW ACO 644 N> (No. 1), <HCW ACO 754 N> (No. 1), <HCW ACO 978 N> (No. 1), <HCW ACO 1126 N> (Nos 1-2), <HCW ACO 1775 N> (No. 1), <HCW ACO 1795 N> (Nos 1-9), <HCW ACO 2029 N> (Nos 1-5), <HCW ACO 2052 N> (No. 1), <HCW ACO 2142N> (Nos 1-9).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HCW2000]
[HCW2000]	(Hunter+Churchwell+Watson+, 2000)= (SMM)
Write:	<<[HCW2000] IRAS HHMMm+DDMM SMM N>> <<[HCW2000] Sgr C SMM>>
N:	4+5+1
Object:	(Submm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Sub-millimeter sources in IRAS 18097-1825, IRAS 18317-0757, and Sgr C.
in source:	IRAS 18097-1825
in source:	IRAS 18317-0757
in source:	NAME Sgr C
Ref:	=2000AJ....119.2711H
by	HUNTER T.R. , CHURCHWELL E., WATSON C., COX P., BENFORD D.J., ROELFSEMA P.R.
	Astron. J., 119, 2711-2727 (2000)
	350 micron images of massive star formation regions.
o	Table 1A: IRAS 17574-2304 misprint for 17574-2403. Table 3: Masers are not in SIMBAD.
o	Table 1: <[HCW2000] Sgr C SMM> N=1. Table 2: <[HCW2000] IRAS 18097-1825 SMM N> (Nos 1-4), <[HCW2000] IRAS 18317-0757 SMM N> (Nos 1-2).
Ref:	=2004ApJ...606..929H
by	HUNTER T.R. , ZHANG Q., SRIDHARAN T.K.
	Astrophys. J., 606, 929-942 (2004)
	IRAS 18317-0757: a cluster of embedded massive stars and protostars.
o	Table 1, Fig.2: <[HCW2000] IRAS 18317-0757 SMM N> (Nos 3-5) added. Table 5: <[HZS2004] C18O NN> (Nos 1-26). Table 7: <[HZS2004] Star NNN> N=44 among 123.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCW2001]
[HCW2001]	(Hyman+Calle+Weiler+, 2001)
Write:	<<[HCW2001] NNa>>
N:	17+7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-7) are discrete radio-sources in NGC 4258, (Nos 13-17) are background sources, (Nos 16a-16d) and (Nos 17a-17c) forming clusters 16 and 17.
in source:	NGC 4258
Ref:	=2001ApJ...551..702H
by	HYMAN S.D. , CALLE D., WEILER K.W., LACEY C.K., VAN DYK S.D., SRAMEK R.
	Astrophys. J., 551, 702-711 (2001)
	Radio continuum imaging of the spiral galaxy NGC 4258.
o	Tables 1, 2: <[HCW2001] NNa> (Nos 1-17, 16a-16d, 17a-17c).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HCW2013]
[HCW2013]	(Hodge+Carilli+Walter+, 2013)
Write:	<<[HCW2013] NN>> <<[HCW2013] JHHMMSS.ss+DDMMSS.s>>
N:	11+4
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLA CO(2-1) line observations of N=11+4 radio sources in the GOODS-N field.
in source:	NAME GOODS-N Field
Ref:	=2013ApJ...776...22H
by	HODGE J.A. , CARILLI C.L., WALTER F., DADDI E., RIECHERS D.
	Astrophys. J., 776, 22 (2013)
	High-resolution spectroscopic imaging of CO in a z = 4.05 proto-cluster.
o	Fig. 5: <[HCW2013] NN> (Nos 1-11) = <[HCW2013] JHHMMSS.ss+DDMMSS.s> N=11. Fig. 8: <[HCW2013] JHHMMSS.ss+DDMMSS.s> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HD
HD	(H. Draper)= (HDE)
Write:	<<HD NNNNNN>> <<HD NNNNNNA>> <<HD NNNNNNAA>> <<HD NNN NNN>> (not recognised by Simbad, but found in literature) <<HD NNN NNNA>> <<HD NNN NNNAA>>
N:	359083+?
Object:	* (SIMBAD class: Star)
Stat.	in SIMBAD: The main part, not Extension
Note:	1918-1924, Ann. Astr. Obs. Harvard College, Vol. 91-99. Reprinted by Bell and Howell. Corrected version available on magnetic tape and microfiche at CDS Strasbourg. Continued by HDE, all are 'HD NNNNNN' in Simbad. (Nos 1-225300) = HD , (Nos 225301-359083) = HDE . The suffix AA indicates a multiple star and the suffix A indicates a component in a multiple star.
Ref:	=1918AnHar..91....0C
by	CANNON A.J. , PICKERING E.C.
	Ann. Astron. Obs. Harvard Coll., -1-None (1918)
	Corrected version available on magnetic tape and microfiche at CDS Strasbourg Henry Draper Catalogue.
o	<HD NNNNNN> (Nos 1-225300)
Ref:	=1925AnHar.100....1C
by	CANNON A.J.
	AnHar, 100, 1-16 (1925)
	The Henry Draper extension. (No. 1).
o	<HD NNNNNN> (Nos 225301-228300).
Ref:	=1925AnHar.100...17C
by	CANNON A.J.
	AnHar, 100, 17-32 (1925)
	The Henry Draper extension. (No.2).
o	<HD NNNNNN> (Nos 228301-231300).
Ref:	=1927AnHar.100...33C
by	CANNON A.J.
	AnHar, 100, 33-48 (1927)
	The Henry Draper extension. (No.3).
o	<HD NNNNNN> (Nos 231301-236300).
Ref:	=1928AnHar.100...49C
by	CANNON A.J.
	AnHar, 100, 49-60 (1928)
	The Henry Draper extension. (No.4).
o	<HD NNNNNN> (Nos 236301-240500).
Ref:	=1931AnHar.100...61C
by	CANNON A.J.
	AnHar, 100, 61-203 (1931)
	The Henry Draper extension. (No.5).
o	<HD NNNNNN> (Nos 240501-268600).
Ref:	=1936AnHar.100..205C
by	CANNON A.J.
	AnHar, 100, 205-226 (1936)
	The Henry Draper extension. (No.6).
o	<HD NNNNNN> (Nos 268601-272150).
Ref:	=1949AnHar.112....1C
by	CANNON A.J. , MAYALL M.W.
	Ann. Astron. Obs. Harvard Coll., 112, 1-295 (1949)
	The Annie J. Cannon Memorial Volume of the Henry Draper Extension.
o	(The Henry Draper extension. II.)
o	<HD NNNNNN> (Nos 272151-359083)
Ref:	=1991A&AS...88..277R
by	ROESER S. , BASTIAN U., WIESE K.
	Astron. Astrophys., Suppl. Ser., 88, 277-280 (1991)
	The second Henry Draper extension: spectral types, magnitudes and precise positions for 10639 stars.
o	<HD NNNNNN> (Nos 332335-342973)
Ref:	=1995A&AS..110..367N
by	NESTEROV V.V. , KUZMIN A.V., ASHIMBAEVA N.T., VOLCHKOV A.A., ROESER S., BASTIAN U.
	Astron. Astrophys., Suppl. Ser., 110, 367-370 (1995)
	The Henry Draper Extension Charts: A catalogue of accurate positions, proper motions, magnitudes and spectral types of 86933 stars.
o	<HD NNNNNN> N=86933
=E=	Catalogue in electronic form as <III/135/>
=E=	Catalogue in electronic form as <III/182/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HD
HD	(H. Draper)
Write:	<<HD NNNNNNa>> <<HD NNNNNNAa>> <<HD NNN NNNa>> (not recognised by Simbad, but found in literature) <<HD NNN NNNAa>>
Object:	Planet (SIMBAD class: Planet = Extra-solar Planet)
Note:	Suffix a added to the formats for the HD stars, to follow in SIMBAD the usage found in the literature.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HD2002]
[HD2002]	(Herbig+Dahm, 2002)
Write:	<<[HD2002] Star NNN>> <<[HD2002] IR N>> <<[HD2002] Cloud A>>
N:	380+310+7+4
Object:	* + (IR) + Cloud (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 1: N=380 stars, pre-main sequence candidate, in IC 5146. Table 2: N=310 stars, pre-main sequence candidate, in the area of BD +46 3471. Table 10: N=7 bright NIR sources. Table 11: N=4 clouds.
in source:	IC 5146
Ref:	=2002AJ....123..304H
by	HERBIG G.H. , DAHM S.E.
	Astron. J., 123, 304-327 (2002)
	The young cluster IC 5146.
o	Tables 1, 2: <[HD2002] Star NNN> (Nos 1-380, 400-710). Tables 1, 2: <IfAHA NNN> (Nos 104-186) added. Table 10: <[HD2002] IR N> (Nos 1-7). Table 11: <[HD2002] Cloud A> (Nos A-D).
=E=	Catalogue in electronic form as J/AJ/123/304
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HD83]
[HD83]	(Hoessel+Danielson, 1983) (Not yet in Simbad)
Write:	<<[HD83] NNN>>
N:	84
Object:	* (SIMBAD class: Star)
Note:	See also: [HM82], [HSD83], [HD84], [HA86]
in source:	GRDG 8
Ref:	=1983ApJ...271...65H
by	HOESSEL J.G. , DANIELSON G.E.
	Astrophys. J., 271, 65-69 (1983)
	Photometry of resolved galaxies. III. GR 8.
o	Table 1: objects are not in SIMBAD
o	Table 1: <[HD83] NNN> (Nos 100-183)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HD84]
[HD84]	(Hoessel+Danielson, 1984) (Not yet in Simbad)
Write:	<<[HD84] Ho I NNN>> <<[HD84] Ho II NNN>>
N:	279+468
Object:	* (SIMBAD class: Star)
Note:	* in Holmberg I galaxy, format 'Ho I NNN', (Nos 100-378). * in Holmberg II galaxy, format 'Ho II NNN', (Nos 100-567). See also: [HM82], [HSD83], [HD83], [HA86]
in source:	Holmberg I = DDO 63
in source:	Holmberg II = DDO 50
Ref:	=1984ApJ...286..159H
by	HOESSEL J.G. , DANIELSON G.E.
	Astrophys. J., 286, 159-170 (1984)
	Photometry of resolved galaxies. IV. Holmberg I and Holmberg II.
o	Tables 1, 2: objects are not in SIMBAD
o	Table 1: <[HD84] Ho I NNN> (Nos 100-378), Table 2: <[HD84] Ho II NNN> (Nos 100-567)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HD90]
[HD90]	(Hummel+Dettmar, 1990)
Write:	<<[HD90] NN>>
N:	12
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 1.49GHz continuum observations of NGC 4631.
in source:	NGC 4631
Ref:	=1990A&A...236...33H
by	HUMMEL E. , DETTMAR R.-J.
	Astron. Astrophys., 236, 33-46 (1990)
	Radio observations and optical photometry of the edge-on spiral galaxy NGC 4631.
o	Table 4: <[HD90] NN> (Nos 1-12).
Details on Acronym: [HD93]
[HD93]	(Hodapp+Deane, 1993)
Write:	<<[HD93] NN>>
N:	47
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Rem:	Plate
in source:	Orion Nebula:LDN 1641 = LDN 1641
Ref:	=1993ApJS...88..119H
by	HODAPP K.-W. , DEANE J.
	Astrophys. J., Suppl. Ser., 88, 119-135 (1993)
	Star formation in the L1641 north cluster.
o	<[HD93] NN> N=47
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HDB84]
[HDB84]	(Henry+DePoy+Becklin, 1984)= (IRR)
Write:	<<[HDB84] IRR N>>
N:	4
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Map in Fig. 1
in source:	NAME Gal Center
Ref:	=1984ApJ...285L..27H
by	HENRY J.P. , DEPOY D.L., BECKLIN E.E.
	Astrophys. J., 285, 27-30 (1984)
	The location of infrared sources in the Galactic Center from a deep 1 micron CCD image.
o	Table 1: <[HDB84] IRR N> (Nos 1-4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HDC2009]
[HDC2009]	(Hagele+Diaz+Cardaci+, 2009)
Write:	<<[HDC2009] ANNa>> <<[HDC2009] R4alpha>>
N:	86
Object:	Star Forming Region (SIMBAD class: Association = Association of Stars)
Note:	WHT ISIS observations of circumnuclear star-forming regions and the nucleus of the spiral galaxy NGC 2903. Use of archival HST WFPC2 data.
in source:	NGC 2903
Ref:	=2009MNRAS.396.2295H
by	HAGELE G.F. , DIAZ A.I., CARDACI M.V., TERLEVICH E., TERLEVICH R.
	Mon. Not. R. Astron. Soc., 396, 2295-2312 (2009)
	On the derivation of dynamical masses of the stellar clusters in the circumnuclear region of NGC2903.
o	Table 4: <[HDC2009] ANNa> N=89 among (Nos R1a-R1d, R2, R2a-R2d, R12a-R12v, R4, R4a-R4z, R7, R7a-R7z, N, Na-Nb), <[HDC2009] R4α> N=1.
=E=	Catalogue in electronic form as <J/MNRAS/396/2295/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HDC2010]
[HDC2010]	(Hagele+Diaz+Cardaci+, 2010) (Not yet in Simbad)
Write:	<<[HDC2010] NGC 3310 ANN>> <<[HDC2010] ANNa>> <<[HDC2010] RNNggg>>
N:	12+113
Object:	Star Forming Region + Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	WHT ISIS observations of circumnuclear star-forming regions and the nucleus of the spiral galaxy NGC 3310.
in source:	NGC 3310
Ref:	=2010MNRAS.402.1005H
by	HAGELE G.F. , DIAZ A.I., CARDACI M.V., TERLEVICH E., TERLEVICH R.
	Mon. Not. R. Astron. Soc., 402, 1005-1026 (2010)
	The circumnuclear environment of the peculiar galaxy NGC3310.
o	Fig. 1, Table 2: <[HDC2010] ANN> (Nos R1-R2, R4-R7, R10, S6, N, J, X, Y). Fig. 10, Table 4: <[HDC2010] ANNa> N=113 among (Nos R1, R1a, R2, R2a-2b, R4, R4a-z, R5, R5a-5g, R6, R6a-6m, S6, S6a-6h, R7, R7a-7z, R10, R10a-n, N, Na), <[HDC2010] RNNalf> (Nos R4alf-R4del, R7alf-R7bet).
=E=	Catalogue in electronic form as <J/MNRAS/402/1005/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HDD2012]
[HDD2012]	(Houghton+Davies+Dalla Bonta+, 2012)
Write:	<<[HDD2012] Phot NNNN>> <<[HDD2012] Spec NNNN>>
N:	532+76
Object:	G (SIMBAD class: Galaxy)
Note:	Gemini North GMOS and HST ACS observations of N=532 galaxies in Abell 1689.
in source:	ACO 1689
Ref:	=2012MNRAS.423..256H
by	HOUGHTON R.C.W. , DAVIES R.L., DALLA BONTA E., MASTERS R.
	Mon. Not. R. Astron. Soc., 423, 256-283 (2012)
	Data and two-dimensional scaling relations for galaxies in Abell 1689: a hint of size evolution at z ~ 0.2.
o	Table 3: <[HDD2012] Phot NNNN> N=532 among (Nos 2-1694), <[HDD2012] Spec NNNN> N=76 among (Nos 14-1164).
=E=	Catalogue in electronic form as J/MNRAS/423/256
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HDE
HDE	(H. Draper, Extension)
====>	Equivalent to: HD
Details on Acronym: HDF
HDF	(Hubble Deep Field)
*****	Avoid the usage of HDF, prefer [FKR97]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDF
HDF	(Hubble Deep Field)
*****	Avoid the usage of HDF, prefer [HBK96]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDF
HDF	(Hubble Deep Field)
*****	Avoid the usage of HDF, prefer [HCB98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDF
HDF	(Hubble Deep Field)
*****	Avoid the usage of HDF, prefer [HSD98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDF
HDF	(Hubble Deep Field)
*****	Avoid the usage of HDF, prefer [LKG97]
Details on Acronym: HDF
HDF	(Hubble Deep Field)
*****	Avoid the usage of HDF, prefer [MM2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDF
HDF	(Hubble Deep Field)
*****	Avoid the usage of HDF, prefer [MS98b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDF
HDF	(Hubble Deep Field)
*****	Avoid the usage of HDF, prefer [PGG97]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDF
HDF	(Hubble Deep Field)
*****	Avoid the usage of HDF, prefer [SGD96]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDF
HDF	(Hubble Deep Field)
*****	Avoid the usage of HDF, prefer [VAE96]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDF
HDF	(Hubble Deep Field)
*****	Avoid the usage of HDF, prefer [WBD96]
Origin	of the Acronym: L (1998ApJ...505L..95W)
Details on Acronym: [HDF2001]
[HDF2001]	(Haberl+Dennerl+Filipovoc+, 2001)
Write:	<<[HDF2001] N>> <<[HDF2001] JHHMM.m+DDMM>>
N:	9
Object:	(Hard X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	N=9 Hard X-ray sources revealed by XMM-Newton first images. Table 2: The authors indicate: 'the coordinates in Table 2 should be regarded as preliminary'. The JHHMM.m+DDMM format used in the the paper is calculated from these coordinates.
Ref:	=2001A&A...365L.208H
by	HABERL F. , DENNERL K., FILIPOVIC M.D., ASCHENBACH B., PIETSCH W., TRUEMPER J.
	Astron. Astrophys., 365, 208-211 (2001)
	AGN in the XMM-Newton first-light image as probes for the interstellar medium in the LMC.
o	Table 2, Fig.1: <[HDF2001] N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HDF2018]
[HDF2018]	(Harris+Drew+Farnhill+, 2018)
Write:	<<[HDF2018] NNN.NN.NNN>> <<[HDF2018] 255.13.337a>> <<[HDF2018] 255.13.337b>>
N:	1183
Object:	* (SIMBAD class: Star)
Note:	MMT HectoSpec observations of N=1183 A and F stars.
Ref:	=2018MNRAS.475.1680H
by	HARRIS A. , DREW J.E., FARNHILL H.J., MONGUIO M., GEBRAN M., WRIGHT N.J., DRAKE J.J., SALE S.E.
	Mon. Not. R. Astron. Soc., 475, 1680-1695 (2018)
	A and F stars as probes of outer Galactic disc kinematics.
o	<[HDF2018] NNN.NN.NNN> N=1181, <[HDF2018] 255.13.337a> (Nos a-b).
=E=	Catalogue in electronic form as <J/MNRAS/475/1680/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HDF850
HDF850	(Hubble Deep Field, 850microm.)
*****	Avoid the usage of HDF850, prefer [HSD98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDFFF
HDFFF	(Hubble Deep Field, Flanking Fields)= (Cowie)
Write:	<<HDFFF MMSSs-MMSS>>
N:	2579
Object:	G (SIMBAD class: Galaxy)
Note:	Cowie catalogue of the HDF Flanking Fields. The complete format of galaxies in the catalogue is, in J2000: 12 MM SS.ss +62 MM SS.s. See also Cowie catalogue in the HDF.
Ref:	=1999AJ....117..102B
by	BARGER A.J. , COWIE L.L., TRENTHAM N., FULTON E., HU E.M., SONGAILA A., HALL D.
	Astron. J., 117, 102-110 (1999)
	Constraints on the early formation of field elliptical galaxies.
o	cowie catalog: <Cowie NNN> (Nos 0-183). hff catalog: <HDFFF MMSSs-MMSS> N=2579.
=E=	Catalogue in electronic form as J/AJ/117/102
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HDFN
HDFN	(Hubble Deep Field, North)
*****	Avoid the usage of HDFN, prefer [BIF2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDFN
HDFN	(Hubble Deep Field, North)
*****	Avoid the usage of HDFN, prefer [BIT2005]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDFS
HDFS	(Hubble Deep Field, South)
*****	Avoid the usage of HDFS, prefer [BBH99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDFS
HDFS	(Hubble Deep Field, South)= (HDFS)
*****	Avoid the usage of HDFS, prefer [FHP2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDFS
HDFS	(Hubble Deep Field, South)
*****	Avoid the usage of HDFS, prefer [GBB2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDFS
HDFS	(Hubble Deep Field, South)
Write:	<<HDFS JHHMMSS.ss+DDMMSS.s>>
N:	2657
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	WHST WFPC2 observations of HDFS. See also [CDD2000].
in source:	NAME HDFS
Ref:	=2000AJ....120.2747C
by	CASERTANO S. , DE MELLO D.F., DICKINSON M., FERGUSON H.C., FRUCHTER A.S., GONZALEZ-LOPEZLIRA R.A., HEYER I., HOOK R.N., LEVAY Z., LUCAS R.A., MACK J., MAKIDON R.B., MUTCHLER M., SMITH T.E., STIAVELLI M., WIGGS M.S., WILLIAMS R.E.
	Astron. J., 120, 2747-2824 (2000)
	WFPC2 observations of the Hubble Deep Field South.
o	Table 6: <[CDD2000] NNNNN> N=2656 among (Nos 1-10719) = <[CDD2000] HDFS JHHMMSS.ss+DDMMSS.s> N=2656 = <HDFS JHHMMSS.ss+DDMMSS.s> N=2656.
=E=	Catalogue in electronic form as J/AJ/120/2747
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDFS
HDFS	(Hubble Deep Field, South)
*****	Avoid the usage of HDFS, prefer [LFR2003]
Origin	of the Acronym: L (2005MNRAS.357.1348W)
Details on Acronym: HDFS
HDFS	(Hubble Deep Field, South)
*****	Avoid the usage of HDFS, prefer [RFF2001]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDFS
HDFS	(Hubble Deep Field, South)
*****	Avoid the usage of HDFS, prefer [RFR2001]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDFS
HDFS	(Hubble Deep Field, South)
*****	Avoid the usage of HDFS, prefer [SGC2001]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDFSMM
HDFSMM	(HDF, SMM)
*****	Avoid the usage of HDFSMM, prefer [BCH2002]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDFSPAR
HDFSPAR	(Hubble Deep Field, Parallel field)
*****	Avoid the usage of HDFSPAR, prefer [BIT2005]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HDFX
HDFX	(HDF, X)
*****	Avoid the usage of HDFX, prefer [HBG2001]
Origin	of the Acronym: L (2003AJ....125.1236D)
Details on Acronym: [HDJ98]
[HDJ98]	(Hawkins+Ducourant+Jones+, 1998)
Write:	<<[HDJ98] NNN>> <<[HDJ98] DNN>>
N:	31+5
Object:	Brown Dwarf (SIMBAD class: Star)
Note:	First results from a survey for low-mass stars and brown dwarfs. Table 1: Photometric sequence, N=31 among N>222 Table 2: Brown Dwarf candidates, DNN, N=5 among N>12, the best candidates are D4, D7 and D12.
Ref:	=1998MNRAS.294..505H
by	HAWKINS M.R.S. , DUCOURANT C., JONES H.R.A., RAPAPORT M.
	Mon. Not. R. Astron. Soc., 294, 505-512 (1998)
	A new population of brown dwarfs.
o	M18 = [HB88] M18
o	Table 1: <[HDJ98] NNN> N=31 among (Nos 8-222). Table 2: <[HDJ98] DNN> N=5 among (Nos D01-D12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HDL95]
[HDL95]	(Heckman+Dahlem+Lehnert+, 1995)
Write:	<<[HDL95] source N>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI and KPNO 4m telescope observations of NGC 1569. 2 bright point sources are observed.
in source:	NGC 1569
Ref:	=1995ApJ...448...98H
by	HECKMAN T.M. , DAHLEM M., LEHNERT M.D., FABBIANO G., GILMORE D., WALLER W.H.
	Astrophys. J., 448, 98-118 (1995)
	An X-ray and optical study of the dwarf galaxy NGC 1569 : evidence for a starburst-driven outflow.
o	Table 2: ridge, halo, blob are not objects in SIMBAD.
o	Table 2: <[HDL95] source N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HDL96]
[HDL96]	(Hoffman+Dickey+Lu+, 1996)
Write:	<<[HDL96] FFF NNN>>
N:	1268
Object:	G (SIMBAD class: Galaxy)
Note:	N=1268 galaxies format 'FFF NNN', in 17 fields 'FFF' (CGCG fields)
Ref:	=1996ApJ...473..822H
by	HOFFMAN G.L. , DICKEY J.M., LU N.Y., FROMHOLD-TREU R.
	Astrophys. J., 473, 822-827 (1996)
	A Minnesota automated plate scanner catalog of galaxies behind the Virgo cluster and toward its antipode.
o	(Erratum) Erratum vol. 480, p. 447
o	table 2 : galaxy 0128+424 not identified
o	Table 3: <[HDL96] FFF NNN> N=1268
=E=	Catalogue in electronic form as J/ApJ/473/822
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HDM
HDM	(Hadfield+van Dyk+Morris+)
Write:	<<HDM NN>>
Object:	WR* (SIMBAD class: WolfRayet* = Wolf-Rayet)
Stat:	is completely incorporated in Simbad
Note:	CTIO 4m Blanco telescope RCSpec observations. Additional NIR spectroscopy at the ARC 3.5m and IRTF 3.0m telescopes.
Ref:	=2007MNRAS.376..248H
by	HADFIELD L.J. , VAN DYK S.D., MORRIS P.W., SMITH J.D., MARSTON A.P., PETERSON D.E.
	Mon. Not. R. Astron. Soc., 376, 248-262 (2007)
	Searching for hidden Wolf-Rayet stars in the Galactic plane - 15 new Wolf-Rayet stars.
o	In chap. 3.1 : Standard star LTT 62648 not identified, it could be LTT 6248.
o	Table 2: <HDM NN> (Nos 1-15).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HDM2017]
[HDM2017]	(Hsu+Desai+Murphy+, 2017)
Write:	<<[HDM2017] HHMM-N>> <<[HDM2017] 0416-3-N>>
N:	14+2
Object:	smm G + (Rad) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	JCMT SCUBA-2 and VLA observations of N=14 submillimeter galaxies and N=2 radio sources in three galaxy cluster fields (MCS J0416.1-2403, MCS J0717.5+3745, and MCS J1149.5+2223).
in source:	MCS J0416.1-2403
in source:	ClG J0717+3745 = MCS J0717.5+3745
in source:	MCS J1149.5+2223
Ref:	=2017ApJ...840...29H
by	HSU L.-Y. , DESAI V., MURPHY E.J., COWIE L.L., HEYWOOD I., MOMJIAN E., BARGER A.J., SMAIL I.
	Astrophys. J., 840, 29-29 (2017)
	The Hawaii SCUBA-2 Lensing Cluster Survey: radio-detected submillimeter galaxies in the HST Frontier Fields.
o	Fig. 3, Table 4: <[HDM2017] HHMM-N> (Nos 0416-1 to 0416-4, 0717-1 to 0717-4, 1149-1 to 1149-6), <[HDM2017] 0416-3-N> (Nos 3-1 to 3-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HDN
HDN	(Hodge, Dark Nebula)
*****	Avoid the usage of HDN, prefer [H74]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [HDN2000]
[HDN2000]	(Hagiwara+Diamond+Nakai+, 2000)
Write:	<<[HDN2000] CN(WW)>>
N:	6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLBA observations. Radio structure of NGC 5793.
in source:	NGC 5793
Ref:	=2000A&A...360...49H
by	HAGIWARA Y. , DIAMOND P.J., NAKAI N., KAWABE R.
	Astron. Astrophys., 360, 49-56 (2000)
	Probing circumnuclear molecular gas in NGC 5793 with OH absorption.
o	Calibrator J1507-168 (J omitted by author) = RORF 1504-166
o	Table 2, Figs 1, 2: <[HDN2000] CN(WW)> (Nos C1(C), C1(NE), C1(SW), C2(C), C2(W), C2(E)).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HDP2017]
[HDP2017]	(Huelamo+De Gregorio-Monsalvo+Palau+, 2017)
Write:	<<[HDP2017] B30-SBNN>>
N:	17
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	APEX SABOCA 350µm continuum observations of N=17 submillimeter sources in the southern part of the Barnard 30 dark cloud. See also [BDH2018].
in source:	Barnard 30
Ref:	=2017A&A...597A..17H
by	HUELAMO N. , DE GREGORIO-MONSALVO I., PALAU A., BARRADO D., BAYO A., RUIZ M.T., ZAPATA L., BOUY H., MORATA O., MORALES-CALDERON M., EIROA C., MENARD F.
	Astron. Astrophys., 597A, 17-17 (2017)
	A search for pre- and proto-brown dwarfs in the dark cloud Barnard 30 with ALMA.
o	Table 2: <[HDP2017] B30-SBNN> (Nos SB01-SB17).
o	Paragraph 3.2 Planck source G192.65-11.70 not identified.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HDR2005]
[HDR2005]	(Homeier+Demarco+Rosati+, 2005)
Write:	<<[HDR2005] NNNNN>>
N:	24
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	HST ACS and VLT-FORS observations of the cluster ClG J0152-1357. See also [DRL2005].
in source:	ClG J0152-1357 = RX J0152.7-1357
Ref:	=2005ApJ...621..651H
by	HOMEIER N.L. , DEMARCO R., ROSATI P., POSTMAN M., BLAKESLEE J.P., BOUWENS R.J., BRADLEY L.D., FORD H.C., GOTO T., GRONWALL C., HOLDEN B., JEE M.J., MARTEL A.R., MEI S., MENANTEAU F., ZIRM A., CLAMPIN M., HARTIG G.F., ILLINGWORTH G.D., ARDILA D.R., BARTKO F., BENITEZ N., BROADHURST T.J., BROWN R.A., BURROWS C.J., CHENG E.S., CROSS N.J.G., FELDMAN P.D., FRANX M., GOLIMOWSKI D.A., INFANTE L., KIMBLE R.A., KRIST J.E., LESSER M.P., MEURER G.R., MILEY G.K., MOTTA V., SIRIANNI M., SPARKS W.B., TRAN H.D., TSVETANOV Z.I., WHITE R.L., ZHENG W.
	Astrophys. J., 621, 651-662 (2005)
	The transformation of cluster galaxies at intermediate redshift.
o	Table 1, col(2): <[HDR2005] NNNNN> N=24 among (Nos 717 -10871).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HDS86]
[HDS86]	(Huang+Dickman+Snell, 1986)
Write:	<<[HDS86] IC 443A>> <<[HDS86] IC 443AN>>
N:	8+6
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Clumps A-H in IC 443. [HDS86] IC 443B and IC 443C correspond to the 2 shocked positions B and C in DeNoyer (1979ApJ...232L.165D). The position A of DeNoyer did not show a perceptible signature in the authors map. These objects are often found in the literature as 'IC 443A' to 'IC 443H'. Subclumps (B1-B4) and (G1-G2) in clumps B and G added by Tauber+
in source:	IC 443
Ref:	=1986ApJ...302L..63H
by	HUANG Y.-L. , DICKMAN R.L., SNELL R.L.
	Astrophys. J., 302, 63-66 (1986)
	IRAS sources associated with shocked gas regions in IC 443.
o	Fig.2: <[HDS86] IC 443A> (Nos IC 443A to IC 443G)
Ref:	=1992ApJ...400..203D
by	DICKMAN R.L. , SNELL R.L., ZIURYS L.M., HUANG Y.-L.
	Astrophys. J., 400, 203-213 (1992)
	Structure and kinematics of dense gas associated with the supernova remnant IC 443.
o	Table 1: <[HDS86] IC443H> added
Ref:	=1994ApJ...421..570T
by	TAUBER J.A. , SNELL R.L., DICKMAN R.L., ZIURYS L.M.
	Astrophys. J., 421, 570-580 (1994)
	High-resolution images of shocked molecular clumps in the supernova remnant IC 443.
o	Tables 1, 2: <[HDS86] IC 443AN> (Nos IC443B1 to IC443B4, IC443G1 to IC443G2)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HDV2021]
[HDV2021]	(Healy+Deb+Verheijen+, 2021)
Write:	<<[HDV2021] NNN>>
N:	219
Object:	HI G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	MeerKAT radio continuum and HI spectral line observations of N=219 galaxies in the field of the galaxy cluster Abell 2626.
in source:	ACO 2626
Ref:	=2021A&A...654A.173H
by	HEALY J. , DEB T., VERHEIJEN M.A.W., BLYTH S.-L., SERRA P., RAMATSOKU M., VULCANI B.
	Astron. Astrophys., 654A, 173-173 (2021)
	MeerKAT 21-cm H I imaging of Abell 2626 and beyond.
o	Table A.1: <[HDV2021] NNN> (Nos 1-219).
=E=	Catalogue in electronic form as <J/A+A/654/A173/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: HDW
HDW	(Hartl+Dengel+Weinberger)= (HtDe)
Write:	<<PN HDW NN>>
N:	13
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	The PN are not numbered by the authors, but found numbered in the literature.
Ref:	=1983MitAG..60..325H
by	HARTL H. , DENGEL J., WEINBERGER R.
	Mitt. Astron. Gesellschaft, 60, 325-327 (1983)
	Alte Planetarische Nebel : neue Kandidaten.
o	The PN are not numbered by authors, but found numbered in literature.
o	Table 1: <PN HDW NN> (Nos 1-13).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HDW2002]
[HDW2002]	(Hofner+Delgado+Whitney+, 2002)
Write:	<<[HDW2002] W3 AN>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
in source:	W 3
Ref:	=2002ApJ...579L..95H
by	HOFNER P. , DELGADO H., WHITNEY B., CHURCHWELL E., LINZ H.
	Astrophys. J., 579, 95-98 (2002)
	X-ray detection of the ionizing stars in ultracompact H II regions.
o	Table 1: <[HDW2002] W3 DN> (Nos D1-D3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HE
HE	(Hamburg-ESO Survey)
Write:	<<HE HHMM+DDMMa>>
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	1st reference: First ref. from the Hamburg-ESO survey, N=1.
Ref:	=1991A&A...247L..17W
by	WISOTZKI L. , WAMSTEKER W., REIMERS D.
	Astron. Astrophys., 247, 17-20 (1991)
	Discovery of a new bright southern QSO.
o	<HE HHMM-DDMM> First ref. from the Hamburg-ESO survey, N=1
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: He
He	(Henize)
*****	Avoid the usage of He, prefer Hen
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HE2000]
[HE2000]	(Hutchings+Edwards, 2000)
Write:	<<[HE2000] N>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=4 radio-sources in the field of 1E 0839.8+2938.
Ref:	=2000AJ....119.1100H
by	HUTCHINGS J.B. , EDWARDS L.
	Astron. J., 119, 1100-1110 (2000)
	Galaxy population properties in the rich clusters MS 0839.8+2938, MS 1224.7+2007, and MS 1231.3+1542.
o	Table 3: <[HE2000] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HE2QS
HE2QS	(HeII Quasar Survey)
Write:	<<HE2QS JHHMM+DDMM>>
N:	9
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	HST COS and STIS observations of HeII-transparent quasars, as part of the HeII Quasar Survey (HE2QS).
Ref:	=2017ApJ...847...81S
by	SCHMIDT T.M. , WORSECK G., HENNAWI J.F., PROCHASKA J.X., CRIGHTON N.H.M.
	Astrophys. J., 847, 81-81 (2017)
	Statistical detection of the He II transverse proximity effect: evidence for sustained quasar activity for >25 million years.
o	Table 2: <HE2QS JHHMM+DDMM> N=5. Table 3: <[SWH2017] JDDD.ddddd+DD.ddddd> N=131.
Ref:	=arXiv:1808.05247
Ref:	=arXiv:1810.03391
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HE81]
[HE81]	(Hjellming, 1981)
Write:	<<[HE81] A>>
N:	17
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Objects in the field of GRB 781119
Ref:	=1981ApJ...246L.137H
by	HJELLMING R.M. , EWALD S.P.
	Astrophys. J., 246, 137-140 (1981)
	A search for radio emission associated with the 1978 november 19 γ-ray burster.
o	Table 1: <[HE81] A> (Nos A-Q)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HEA
HEA	(Hardy et al.)
Write:	<<HEA NNNNW>>
N:	1287
Object:	* (SIMBAD class: Star)
Note:	The 'HEA' catalog is described in 1984ApJ...278..592H
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1985A&AS...61..473B
by	BERNAZZANI M. , BUONANNO R., CORSI C.E., HARDY E.
	Astron. Astrophys., Suppl. Ser., 61, 473-482 (1985)
	Magnitudes, colors and positions for bright stars in the Large Magellanic Cloud bar.
o	Table I: <HEA NNNNW> N=1287
=E=	Catalogue in electronic form as J/A+AS/61/473
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HEA2010]
[HEA2010]	(Heiderman+Evans+Allen+, 2010) (Not yet in Simbad)
Write:	<<[HEA2010] JHHMMSS.ss+DDMMSS.ss>>
N:	97
Object:	Suspicious YSO + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Spitzer IRAC and MIPS observations of N=20 large molecular clouds.
Ref:	=2010ApJ...723.1019H
by	HEIDERMAN A. , EVANS II N.J., ALLEN L.E., HUARD T., HEYER M.
	Astrophys. J., 723, 1019-1037 (2010)
	The star formation rate and gas surface density relation in the Milky Way: implications for extragalactic studies.
o	Table 3: <[HEA2010] JHHMMSS.ss+DDMMSS.ss> N=97.
o	In table 6: IRAS20126, IRAS20220 et IRAS23385 are not identified (incomplete format).
=E=	Catalogue in electronic form as <J/ApJ/723/1019/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HEAO
HEAO	(HEAO satellite)
*****	Avoid the usage of HEAO, prefer H
Details on Acronym: HEAO
HEAO	(HEAO satellite)
*****	Avoid the usage of HEAO, prefer 1H
Details on Acronym: HEAO 4-
HEAO 4-	(HEAO satellite, 4th experience)
*****	Avoid the usage of HEAO 4-, prefer H
Details on Acronym: [HEB2019]
[HEB2019]	(Hunter+Elmegreen+Berger, 2019)
Write:	<<[HEB2019] CVnIdwA N>> <<[HEB2019] DDO NNN NN>> <<[HEB2019] F564-V3 N>> <<[HEB2019] IC NNNN NN>> <<[HEB2019] LGS 3 N>> <<[HEB2019] M81dwA 1>> <<[HEB2019] NGC NNNN NNN>> <<[HEB2019] SagDIG N>> <<[HEB2019] UGC 8508 N>> <<[HEB2019] WLM NN>> <<[HEB2019] Haro NN N>> <<[HEB2019] Mrk 178 N>> <<[HEB2019] VII Zw 403 N>>
N:	814
Object:	HI Cloud (SIMBAD class: HI = HI (21cm) Source)
Note:	N=814 discrete HI clouds in 40 dwarf irregular galaxies from the LITTLE THINGS survey. Use of VLA HI data cubes from the LITTLE THINGS survey.
Ref:	=2019AJ....157..241H
by	HUNTER D.A. , ELMEGREEN B.G., BERGER C.L.
	Astron. J., 157, 241-241 (2019)
	H I clouds in LITTLE THINGS dwarf irregular galaxies.
o	Table 2: <[HEB2019] CVnIdwA N>, <[HEB2019] DDO NNN NN>, <[HEB2019] F564-V3 N>, <[HEB2019] IC NNNN NN>, <[HEB2019] LGS 3 N>, <[HEB2019] >, <[HEB2019] M81dwA 1>, <[HEB2019] NGC NNNN NNN>, <[HEB2019] SagDIG N>, <[HEB2019] UGC 8508 N>, <[HEB2019] WLM NN>, <[HEB2019] Haro NN N>, <[HEB2019] Mrk 178 N>, <[HEB2019] VII Zw 403 N>, N=814.
=E=	Catalogue in electronic form as <J/AJ/157/241/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HEC
HEC	(High Extinction Cloud)
Write:	<<HEC GLLL.ll+BB.bb>> <<HEC GLLL.ll+BB.bbA>> <<HEC GLLL.ll+BB.bb MMN>> <<HEC GLLL.ll+BB.bbA MMN>>
N:	226+31+44+11+52+44
Object:	Cloud + Clump (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	IRAM 30m telescope MAMBO 1.2mm observations of infrared dark clouds.
Ref:	=2010A&A...515A..42R
by	RYGL K.L.J. , WYROWSKI F., SCHULLER F., MENTEN K.M.
	Astron. Astrophys., 515A, 42-42 (2010)
	Initial phases of massive star formation in high infrared extinction clouds. I. Physical parameters.
o	Tables 1-2: <HEC GLLL.ll+BB.bbA> N=226+31. Tables 3-5, 7: <HEC GLLL.ll+BB.bbA MMN> N=44+11+52+44.
=E=	Catalogue in electronic form as J/A+A/515/A42
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HED2000]
[HED2000]	(Hackenberg+Eckart+Davies+, 2000) (Not yet in Simbad)
Write:	<<[HED2000] J1836.3CR aN>> <<[HED2000] PKS 0743-006 a>>
N:	8+5
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Fig.11, Table 9: N=8 sources in CEMM J1836.3CR field, all are galaxies. Fig.12, Table 10: N=5 sources in PKS 0743-006 field, 3 galaxies and 2 stars.
Ref:	=2000A&A...363...41H
by	HACKENBERG W. , ECKART A., DAVIES R.I., RABIEN S., OTT T., KASPER M., HIPPLER S., QUIRRENBACH A.
	Astron. Astrophys., 363, 41-61 (2000)
	Near-infrared adaptive optics observations of galaxy clusters: Abell 262 at z=0.0157, J1836.3CR at z=0.414, and PKS 0743-006 at z=0.994.
o	J1836.3CR = CEMM J1836.3CR
o	Fig.11, Table 9: <[HED2000] J1836.3CR aN> (Nos a-g, b2). Fig.12, Table 10: <[HED2000] PKS 0743-006 a> (Nos a-e).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HEF97]
[HEF97]	(Halpern+Eracleous+Forster, 1997)
Write:	<<[HEF97] JHHMMSS.ss+DDMMSS.s>>
N:	2
Object:	(Rad) + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI and optical observations in the field of 1E 0336-24.8. One radio-source '[HEF97] J033812.93-244351.9' and one bright galaxy '[HEF97] J033812.39-244507.8' are found
Ref:	=1997AJ....114.1736H
by	HALPERN J.P. , ERACLEOUS M., FORSTER K.
	Astron. J., 114, 1736-1740 (1997)
	E 0336-248: a new BL Lac object found by an old Einstein.
o	Radiosource = EQ J033812-244351. HII galaxy = EQ J033812-244507
o	<[HEF97] JHHMMSS.ss+DDMMSS.s> N=2
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HeFa
HeFa	(Henize+Fairall)
Write:	<<PN HeFa N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Ref:	=1983IAUS..103..544H
by	HENIZE K.G. , FAIRALL A.P.
	IAU Symp., 103, held at University College, London, U.K. August 9-13, 1982 Ed. by D.R. Flower., 103, 544-None (1983)
	A new planetary nebula with independently determined distance and mass.
o	<PN HeFa 1> N=1
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HeFe
HeFe	(Heckathorn+Fesen+)
*****	Avoid the usage of HeFe, prefer HFG
Details on Acronym: [HEG2001]
[HEG2001]	(Heinke+Edmonds+Grindlay, 2001)
Write:	<<[HEG2001] A>>
N:	7
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of sources in NGC 6652. See also CXOGlb.
Ref:	=2001ApJ...562..363H
by	HEINKE C.O. , EDMONDS P.D., GRINDLAY J.E.
	Astrophys. J., 562, 363-367 (2001)
	Identification of the low-mass X-ray binary and faint X-ray sources in NGC 6652.
o	Table 1: <[HEG2001] A> (Nos A-D) = <CXOGlb JHHMMSS.s+DDMMSS> N=4.
Ref:	=2011ApJ...735...95C
by	COOMBER G. , HEINKE C.O., COHN H.N., LUGGER P.M., GRINDLAY J.E.
	Astrophys. J., 735, 95 (2011)
	The unusual X-ray binaries of the globular cluster NGC 6652.
o	Fig.1, Table 1: <[HEG2001] A> (Nos E-G) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HEG2003]
[HEG2003]	(Heinke+Edmonds+Grindlay+, 2003)= (Ter)
Write:	<<[HEG2003] WNN>> <<[HEG2003] Star N>>
N:	9+2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-I observations of Cl Terzan 5. N=9 sources (Nos W2-W10) detected besides EXO 1745-248. N=2 stars in the error circle of EXO 1745-248.
in source:	Cl Terzan 5
Ref:	=2003ApJ...590..809H
by	HEINKE C.O. , EDMONDS P.D., GRINDLAY J.E., LLOYD D.A., COHN H.N., LUGGER P.M.
	Astrophys. J., 590, 809-821 (2003)
	A Chandra X-ray study of the dense globular cluster Terzan 5.
o	p.811: source S2 of Johnston + 1995 is EQ J174734.4-244558 in SIMBAD.
o	Fig.2, Table 1, col(2): <[HEG2003] WNN> (Nos W2-W10) = Table 1, col(1): <CXOGlb JHHMMSS.s+DDMMSS> N=9, <[HEG2003] Star N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HEH2007]
[HEH2007]	(Hicks+Ellingson+Hoekstra+, 2007)
Write:	<<[HEH2007] soft NN>> <<[HEH2007] hard NN>>
N:	26+18
Object:	soft and hard (X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of the cluster RCS J0224.5-0002.
in source:	RCS J0224.0-0002
Ref:	=2007ApJ...671.1446H
by	HICKS A.K. , ELLINGSON E., HOEKSTRA H., GLADDERS M., YEE H.K.C., BAUTZ M., GILBANK D., WEBB T., IVISON R.
	Astrophys. J., 671, 1446-1455 (2007)
	A multiwavelength analysis of the strong lensing cluster RCS 022434-0002.5 at z=0.778.
o	Table 3: <[HEH2007] soft NN> (Nos 1-26). Table 4: <[HEH2007] hard NN> (Nos 1-18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HEH2008]
[HEH2008]	(Huffenberger+Eriksen+Hansen+, 2008)
Write:	<<[HEH2008] JHHMMSS+DDMMSS>>
N:	8
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	WMAP unresolved point sources.
Ref:	=2008ApJ...688....1H
by	HUFFENBERGER K.M. , ERIKSEN H.K., HANSEN F.K., BANDAY A.J., GORSKI K.M.
	Astrophys. J., 688, 1-11 (2008)
	The scalar perturbation spectral index n_{s}: WMAP sensitivity to unresolved point sources.
o	Table 1: <[HEH2008] JHHMMSS+DDMMSS> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Heiles
Heiles	(Heiles)
*****	Avoid the usage of Heiles, prefer HCl
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HELGA
HELGA	(Herschel Exploitation of Local Galaxy Andromeda)
*****	Avoid the usage of HELGA, prefer [KGF2015]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HELLAS
HELLAS	(High Energy Large Area Survey)
Write:	<<HELLAS NNN>> <<HELLAS NNN.N>>
N:	147
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	BeppoSAX HELLAS catalogue. See also [FLG99].
Ref:	=2001MNRAS.327..771F
by	FIORE F. , GIOMMI P., VIGNALI C., COMASTRI A., MATT G., PEROLA G.C., LA FRANCA F., MOLENDI S., TAMBURELLI F., ANTONELLI L.A.
	Mon. Not. R. Astron. Soc., 327, 771-780 (2001)
	The BeppoSAX High Energy Large Area Survey (HELLAS) - II. Number counts and X-ray spectral properties.
o	Table 2: <HELLAS NNN>, <HELLAS NNN.N>, N=147 among (Nos 6-431).
=E=	Catalogue in electronic form as J/MNRAS/327/771
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HELLAS2XMM
HELLAS2XMM	(High Energy Large Area Survey, XMM-Newton)= (H2XMM)
Write:	<<HELLAS2XMM FFFFNNNNa>> <<HELLAS2XMM JHHMMSS.s+DDMMSS>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Identifications of X-ray sources discovered by XMM-Newton in the 2-10 keV band (HELLAS2XMM 1dF sample). The format 'FFFFNNNN' is always a 8 digits format. In the format, 'FFFF' stands for authors' designation for one of the 15 fields described in 2002ApJ...564..190B (ex.: field 0312 around PKS 0312-77, field 2690 around ACO 2690, field 1580 around G158-100, field 5090 around Mrk 509). See also [CFV2007].
Ref:	=2003A&A...409...79F
by	FIORE F. , BRUSA M., COCCHIA F., BALDI A., CARANGELO N., CILIEGI P., COMASTRI A., LA FRANCA F., MAIOLINO R., MATT G., MOLENDI S., MIGNOLI M., PEROLA G.C., SEVERGNINI P., VIGNALI C.
	Astron. Astrophys., 409, 79-90 (2003)
	The HELLAS2XMM survey. IV. Optical identifications and the evolution of the accretion luminosity in the Universe.
o	Table 1: <HELLAS2XMM FFFFNNNN>, <HELLAS2XMM FFFFNNNNa> = <HELLAS2XMM JHHMMSS.s+DDMMSS>, N=122.
Ref:	=2003A&A...409...65B
by	BRUSA M. , COMASTRI A., MIGNOLI M., FIORE F., CILIEGI P., VIGNALI C., SEVERGNINI P., COCCHIA F., LA FRANCA F., MATT G., PEROLA G.C., MAIOLINO R., BALDI A., MOLENDI S.
	Astron. Astrophys., 409, 65-78 (2003)
	The HELLAS2XMM survey. III. Multiwavelength observations of hard X-ray selected sources in the PKS 0312-77 field.
o	Table 1: <HELLAS2XMM 0312NNNN> N=35 among (Nos NNNN 0003 to 0501).
Ref:	=2007A&A...466...31C
by	COCCHIA F. , FIORE F., VIGNALI C., MIGNOLI M., BRUSA M., COMASTRI A., FERUGLIO C., BALDI A., CARANGELO N., CILIEGI P., D'ELIA V., LA FRANCA F., MAIOLINO R., MATT G., MOLENDI S., PEROLA G.C., PUCCETTI S.
	Astron. Astrophys., 466, 31-40 (2007)
	The HELLAS2XMM survey. VIII. Optical identifications of the extended sample.
o	Table 1, cols(opt. ID): <[CFV2007] JHHMMSS.s+DDMMSS> N=117. Tables 1, 3, 4: <HELLAS2XMM JHHMMSS.s+DDMMSS> N=141.
=E=	Catalogue in electronic form as J/A+A/409/79
=E=	Catalogue in electronic form as J/A+A/466/31
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HELMS
HELMS	(HerMES Large Mode Survey)
*****	Avoid the usage of HELMS, prefer [ACS2016]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HELMS
HELMS	(HerMES Large Mode Survey)
*****	Avoid the usage of HELMS, prefer [NKC2016]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HELP
HELP	(Herschel Extragalactic Legacy Project)
Write:	<<HELP JHHMMSS.sss+DDMMSS.sss>>
N:	∼170 million
Object:	(NIR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	The Herschel Extragalactic Legacy Project (HELP) provides an optical to near-infrared (NIR) selected astronomical catalogue of N∼170 million objects covering 1270 q. deg, based on 51 public surveys. More information available at: http://herschel.sussex.ac.uk/ https://herschel-vos.phys.sussex.ac.uk/
Ref:	=2019MNRAS.490..634S
by	SHIRLEY R. , ROEHLLY Y., HURLEY P.D., BUAT V., CAMPOS VARILLAS M.D.C., DUIVENVOORDEN S., DUNCAN K.J., EFSTATHIOU A., FARRAH D., GONZALEZ SOLARES E., MALEK K., MARCHETTI L., McCHEYNE I., PAPADOPOULOS A., PONS E., SCIPIONI R., VACCARI M., OLIVER S.
	Mon. Not. R. Astron. Soc., 490, 634-656 (2019)
	HELP: a catalogue of 170 million objects, selected at 0.36-4.5 µm, from 1270 °^{2} of prime extragalactic fields.
o	<HELP JHHMMSS.sss+DDMMSS.sss> N~170 million.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HEM2008]
[HEM2008]	(Harayama+Eisenhauer+Martins, 2008)
Write:	<<[HEM2008] NNN>>
N:	256
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT NACO AO-assisted observations of NGC 3603.
in source:	NGC 3603
Ref:	=2008ApJ...675.1319H
by	HARAYAMA Y. , EISENHAUER F., MARTINS F.
	Astrophys. J., 675, 1319-1342 (2008)
	The initial mass function of the massive star-forming region NGC 3603 from near-infrared adaptive optics observations.
o	Center position of NGC 3608 given in table 6 is in error; accurate coordinates as remeasured by F. Eisenhauer are : 11:15:07.337 -61:15:38.19 (private communication).
o	Table 6: <[HEM2008] NNN> (Nos 1-256).
=E=	Catalogue in electronic form as J/ApJ/675/1319
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HEM2018]
[HEM2018]	(Hansen+El-Souri+Monaco+, 2018)
Write:	<<[HEM2018] Sgr NNNNNNN>>
N:	3
Object:	Giant * (SIMBAD class: Star)
Note:	VLT UVES observations of N=3 giant stars in the Sagittarius dwarf galaxy.
in source:	NAME SDG = NAME Sgr Dwarf Galaxy
Ref:	=2018ApJ...855...83H
by	HANSEN C.J. , EL-SOURI M., MONACO L., VILLANOVA S., BONIFACIO P., CAFFAU E., SBORDONE L.
	Astrophys. J., 855, 83-83 (2018)
	Ages and heavy element abundances from very metal-poor stars in the Sagittarius dwarf galaxy.
o	Tables 1-3: <[HEM2018] Sgr NNNNNNN> (Nos 2300225, 2300275, 3600436).
=E=	Catalogue in electronic form as <J/ApJ/855/83/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Hen
Hen	(Henize)= (He) = (Henize) = (Henun) = (LH-alpha)
Write:	<<Hen 1-N>> <<Hen 2-NNN>> <<Hen 3-NNNN>> <<Hen 4-NNN>>
N:	7+468+1929+250
Object:	PN + Em* + * (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	Hen 1-N: N=7 PN. Hen 2-NNN: N=468 PN. Hen 3-NNNN: N=1929 are emission stars, among which 2 are compiled as PN (Nos 1312 and 1333). Hen 4-NNN: S stars from an unpublished list of Henize. Description in 1960AJ......65..491H. N=166 among (Nos 1-236), cross-id. with CSS in 1984PW&SO...3....1S. (Nos 1-205), cross-id. with CSS in 2000A&AS..145...51V.
Ref:	=1961PASP...73..159H
by	HENIZE K.G.
	Publ. Astron. Soc. Pac., 73, 159-162 (1961)
	Seven new planetary nebulae.
o	<Hen 1-N> (Nos 1-1 to 1-7).
Ref:	=1967ApJS...14..125H
by	HENIZE K.G.
	Astrophys. J., Suppl. Ser., 14, 125-153 (1967)
	Observations of southern planetary nebulae.
o	<Hen 2-NNN> (Nos 2-1 to 2-468).
Ref:	=1976ApJS...30..491H
by	HENIZE K.G.
	Astrophys. J., Suppl. Ser., 30, 491-550 (1976)
	Observations of southern emission-line stars.
o	Table 1: <Hen 3-1 to 3-1929>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Hen N
Hen N	(Henize, Nebula)
*****	Avoid the usage of Hen N, prefer LHA 115-N
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Hen N
Hen N	(Henize, Nebula)
*****	Avoid the usage of Hen N, prefer LHA 120-N
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Hen S
Hen S	(Henize, Star)
*****	Avoid the usage of Hen S, prefer LHA 115-S
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Hen S
Hen S	(Henize, Star)
*****	Avoid the usage of Hen S, prefer LHA 120-S
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HenG
HenG	(Henning, 1992)
*****	Avoid the usage of HenG, prefer [H92]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: Henize
Henize	(Henize)
*****	Avoid the usage of Henize, prefer Hen
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Henun
Henun	(Henize, Unpublished)
Origin	of the Acronym: L (1984PW&SO...3....1S)
Details on Acronym: Her
Her	(Herschel)= (Herschel) = (HJ)
Write:	<<** Her NNNN>>
Object:	(SIMBAD class: = Double or Multiple Star)
Auth.:	HERSCHEL J.F.W.
Details on Acronym: Her
Her	(Her-1 field)
*****	Avoid the usage of Her, prefer [MBR95]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Her
Her	(Hercules cluster)
*****	Avoid the usage of Her, prefer [SS78]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HER2000]
[HER2000]	(Hopwood+Evans+Roberts+, 2000)
Write:	<<[HER2000] N>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations of NGC 5779. N=3 point sources. Image in Fig.1.
in source:	NGC 5779
Ref:	=2000MNRAS.316L...5H
by	HOPWOOD M.E.L. , EVANS A., ROBERTS T.P., BURLEIGH M.R., ODENKIRCHEN M., BEARDMORE A.P., O'BRIEN T., JEFFRIES R.D., PENNY A., EYRES S.P.S.
	Mon. Not. R. Astron. Soc., 316, 5-8 (2000)
	A possible detection of diffuse extended X-ray emission in the environment of the globular cluster NGC 6779.
o	Table 2: <[HER2000] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HER2012]
[HER2012]	(Ho+Ebeling+Richard, 2012)
Write:	<<[HER2012] JHHMMSS.ss+DDMMSS.ss>>
N:	72
Object:	G (SIMBAD class: Galaxy)
Note:	Keck-I LRIS and Keck-II DEIMOS spectroscopy of N=72 galaxies in the field of MCS J0140.0-0555.
in source:	MCS J0140.0-0555
Ref:	=2012MNRAS.426.1992H
by	HO I.-T. , EBELING H., RICHARD J.
	Mon. Not. R. Astron. Soc., 426, 1992-2002 (2012)
	An x-ray/optical study of the geometry and dynamics of MACSJ0140.0-0555, a massive post-collision cluster merger.
o	Table 2: <[HER2012] JHHMMSS.ss+DDMMSS.ss> N=72.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HER2013]
[HER2013]	(Hsu+Ebeling H.+Richard, 2013)
Write:	<<[HER2013] JHHMMSS.ss-DDMMSS.s>>
N:	10+64
Object:	G (SIMBAD class: Galaxy)
Note:	Keck I LRIS spectroscopic observations of N=10+64 galaxies in the field of MACS J0358.8-2955.
in source:	ACO 3192
in source:	MCS J0358.8-2955
Ref:	=2013MNRAS.429..833H
by	HSU L.-Y. , EBELING H., RICHARD J.
	Mon. Not. R. Astron. Soc., 429, 833-848 (2013)
	The three-dimensional geometry and merger history of the massive galaxy cluster MACS J0358.8-2955.
o	Tables 2,3: <[HER2013] JHHMMSS.ss+DDMMSS.s> N=10+64.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Herbig
Herbig	(Herbig) (Not yet in Simbad)
Write:	<<Herbig NN>>
N:	33
Object:	RFN (SIMBAD class: RefNeb = Reflection Nebula)
Note:	Tables 3, 4, col(1): (Nos 1-33), Be and Ae stars associated with nebulosity.
Ref:	=1960ApJS....4..337H
by	HERBIG G.H.
	Astrophys. J., Suppl. Ser., 4, 337-368 (1960)
	The spectra of Be and Ae type stars associated with nebulosity.
o	Tables 3 col(2), 6, 13: <Em* LkHA NNN> (Nos 198-205, 208, 210-217, 233-234). Tables 3 and 4 col(1): <Herbig NN> (Nos 1-33).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: Herbig
Herbig	(Herbig)
*****	Avoid the usage of Herbig, prefer LkHA
Origin	of the Acronym: L (2004AJ....127.2659R)
Details on Acronym: HerBS
HerBS	(Herschel Bright Sources)
Write:	<<HerBS NNN>>
N:	209
Object:	High redshift G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	The Herschel Bright Sources (HerBS) sample is a sample of bright, high-redshift Herschel sources detected in the 616.4 square degree H-ATLAS survey. The HerBS sample contains 209 galaxies, selected with a 500µm flux density greater than 80mJy and an estimated redshift greater than 2. The sample consists of a combination of HyLIRGs and lensed ULIRGs during the epoch of peak cosmic star formation.
Ref:	=2018MNRAS.473.1751B
by	BAKX T.J.L.C. , EALES S.A., NEGRELLO M., SMITH M.W.L., VALIANTE E., HOLLAND W.S., BAES M., BOURNE N., CLEMENTS D.L., DANNERBAUER H., DE ZOTTI G., DUNNE L., DYE S., FURLANETTO C., IVISON R.J., MADDOX S., MARCHETTI L., MICHALOWSKI M.J., OMONT A., OTEO I., WARDLOW J.L., VAN DER WERF P., YANG C.
	Mon. Not. R. Astron. Soc., 473, 1751-1773 (2018)
	The Herschel Bright Sources (HerBS): sample definition and SCUBA-2 observations.
o	(Erratum) erratum vol. 494, p. 10 (2020)
o	Table A1: <HerBS NNN> N=209. Cardiff University
=E=	Catalogue in electronic form as <J/MNRAS/473/1751/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: Herbst
Herbst	(Herbst)
*****	Avoid the usage of Herbst, prefer VDBH
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Herbst
Herbst	(Herbst)
*****	Avoid the usage of Herbst, prefer VDBH
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HERMES
HERMES	(Herschel Multi-Tiered Extragalactic Survey) (Not yet in Simbad)
Write:	<<HERMES S-xID24-NNNNNN>> <<HERMES P-NNNNNN>> <<HERMES -xID24-NNNNNN>> (not recognised by Simbad, but found in literature)
N:	554792+282186
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	"Cross-identification" catalogues based on prior Spitzer MIPS 24µm source positions. For more information, visit the HerMES website: http://hedam.lam.fr/HerMES/ See also 4HERMES.
Ref:	=2017yCat.8103....0H
by	HERMES TEAM
	yCat, 8103, 0 (2017)
	Herschel Multi-tiered Extragalactic Survey.
o	spirex24: <HERMES S-xID24-NNNNNN> N=554792 among (Nos 000001-557614). spire250: <4HERMES S250 SF JHHMMSS.s+DDMMSS> N=419928. pacsx24: <HERMES P-NNNNNN> N=282186 among (Nos 0-303041).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HERMES
HERMES	(Herschel Multi-Tiered Extragalactic Survey)
Write:	<<HERMES JHHMMSS.s+DDMMSS>>
N:	about 500000
Object:	G (SIMBAD class: Galaxy)
Note:	Large survey with ESA's Herschel Space Observatory (http://hermes.sussex.ac.uk/)
Auth.:	Seb Oliver
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: 1HERMES
1HERMES	(HerMES catalogues, DR1) (Not yet in Simbad)
*****	Avoid the usage of 1HERMES, prefer [CBB2012]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 1HERMES
1HERMES	(HerMES catalogues, DR1)
Write:	<<1HERMES {S250\|S350\|S500} JHHMMSS.s+DDMMSS>>
N:	?
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Naming convention for the catalogues associated with the initial Herschel SPIRE/SAG-1/HerMES public data release (DR1). The HerMES first data release provides three different catalogue types for each field: SUSSEXtractor (SX) and StarFinder (SF) mono-wavelength catalogues and band-merged xID ones. For more information, see the HerMES official website: http://hermes.sussex.ac.uk/ See also the HeDaM database, available at: http://hedam.oamp.fr/HerMES/ In the format, SNNN refers to the wavelength of the map where the source was identified (S250, S350 or S500 for SPIRE catalogues).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 2HERMES
2HERMES	(HerMES catalogues, DR2)
Write:	<<2HERMES {S250\|S350\|S500} JHHMMSS.s+DDMMSS>>
N:	340968+288754+177487+79860
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Naming convention for the catalogues associated with the second Herschel SPIRE/SAG-1/HerMES public data release (DR2). The HerMES second data release provides three different catalogue types for each field: SUSSEXtractor (SX) and StarFinder (SF) mono-wavelength catalogues and band-merged xID ones. For more information, visit: http://hedam.oamp.fr/HerMES/ In the format, SNNN refers to the wavelength of the map where the source was identified (S250, S350 or S500 for SPIRE catalogues). See also <1HERMES>.
Ref:	=2012MNRAS.424.1614O
by	OLIVER S.J. , BOCK J., ALTIERI B., AMBLARD A., ARUMUGAM V., AUSSEL H., BABBEDGE T., BEELEN A., BETHERMIN M., BLAIN A., BOSELLI A., BRIDGE C., BRISBIN D., BUAT V., BURGARELLA D., CASTRO-RODRIGUEZ N., CAVA A., CHANIAL P., CIRASUOLO M., CLEMENTS D.L., CONLEY A., CONVERSI L., COORAY A., DOWELL C.D., DUBOIS E.N., DWEK E., DYE S., EALES S., ELBAZ D., FARRAH D., FELTRE A., FERRERO P., FIOLET N., FOX M., FRANCESCHINI A., GEAR W., GIOVANNOLI E., GLENN J., GONG Y., GONZALEZ SOLARES E.A., GRIFFIN M., HALPERN M., HARWIT M., HATZIMINAOGLOU E., HEINIS S., HURLEY P., HWANG H.S., HYDE A., IBAR E., ILBERT O., ISAAK K., IVISON R.J., LAGACHE G., LE FLOC'H E., LEVENSON L., FARO B.L., LU N., MADDEN S., MAFFEI B., MAGDIS G., MAINETTI G., MARCHETTI L., MARSDEN G., MARSHALL J., MORTIER A.M.J., NGUYEN H.T., O'HALLORAN B., OMONT A., PAGE M.J., PANUZZO P., PAPAGEORGIOU A., PATEL H., PEARSON C.P., PEREZ-FOURNON I., POHLEN M., RAWLINGS J.I., RAYMOND G., RIGOPOULOU D., RIGUCCINI L., RIZZO D., RODIGHIERO G., ROSEBOOM I.G., ROWAN-ROBINSON M., SANCHEZ PORTAL M., SCHULZ B., SCOTT D., SEYMOUR N., SHUPE D.L., SMITH A.J., STEVENS J.A., SYMEONIDIS M., TRICHAS M., TUGWELL K.E., VACCARI M., VALTCHANOV I., VIEIRA J.D., VIERO M., VIGROUX L., WANG L., WARD R., WARDLOW J., WRIGHT G., XU C.K., ZEMCOV M.
	Mon. Not. R. Astron. Soc., 424, 1614-1635 (2012)
	The Herschel Multi-tiered Extragalactic Survey: HerMES.
o	merge: <2HERMES S250 JHHMMSS.s+DDMMSS> N=340968. sx250: <2HERMES S250 JHHMMSS.s+DDMMSS> N=288754. sx350: <2HERMES S350 JHHMMSS.s+DDMMSS> N=177487. sx500: <2HERMES S500 JHHMMSS.s+DDMMSS> N=79860.
=E=	Catalogue in electronic form as <VIII/95/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: 4HERMES
4HERMES	(HerMES catalogues, DR4)
Write:	<<4HERMES S250 SF JHHMMSS.s+DDMMSS>>
N:	554792+419928+282186
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	This naming convention is for the HerMES DR4 band-merged catalog. In the format, {S250} stands for the SPIRE 250µm filter, and SF stands for StarFinder (SF). For more information, visit: https://irsa.ipac.caltech.edu/data/Herschel/HerMES/overview.html http://hedam.oamp.fr/HerMES/ See also <1HERMES>, 2HERMES.
Ref:	=2017yCat.8103....0H
by	HERMES TEAM
	yCat, 8103, 0 (2017)
	Herschel Multi-tiered Extragalactic Survey.
o	spirex24: <HERMES S-xID24-NNNNNN> N=554792 among (Nos 000001-557614). spire250: <4HERMES S250 SF JHHMMSS.s+DDMMSS> N=419928. pacsx24: <HERMES P-NNNNNN> N=282186 among (Nos 0-303041).
=E=	Catalogue in electronic form as VIII/103
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HerS
HerS	(Herschel Stripe 82 Survey)
Write:	<<HerS DDD.dddddd+DD.dddddd>> <<HerS JHHMMSS.ss+DDMMSS.ss>> <<HerS JHHMMSS.s+DDMMSS>>
N:	32815
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Herschel SPIRE observations of SDSS Stripe 82. Band-merged catalog from the Herschel Stripe 82 Survey (HerS). More information available at: http://www.astro.caltech.edu/hers/.
Ref:	=2014ApJS..210...22V
by	VIERO M.P. , ASBOTH V., ROSEBOOM I.G., MONCELSI L., MARSDEN G., MENTUCH COOPER E., ZEMCOV M., ADDISON G., BAKER A.J., BEELEN A., BOCK J., BRIDGE C., CONLEY A., DEVLIN M.J., DORE O., FARRAH D., FINKELSTEIN S., FONT-RIBERA A., GEACH J.E., GEBHARDT K., GILL A., GLENN J., HAJIAN A., HALPERN M., JOGEE S., KURCZYNSKI P., LAPI A., NEGRELLO M., OLIVER S.J., PAPOVICH C., QUADRI R., ROSS N., SCOTT D., SCHULZ B., SOMERVILLE R., SPERGEL D.N., VIEIRA J.D., WANG L., WECHSLER R.
	Astrophys. J., Suppl. Ser., 210, 22 (2014)
	The Herschel Stripe 82 Survey (HerS): maps and early catalog.
o	catalog: <HerS DDD.dddddd+DD.dddddd> N=32815.
=E=	Catalogue in electronic form as J/ApJS/210/22
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Herschel
Herschel	(Herschel)
*****	Avoid the usage of Herschel, prefer Her
Details on Acronym: Herz
Herz	(Herz)
Write:	<<HERZ NNNNN>>
Object:	* (SIMBAD class: Star)
Note:	From Herz catalog: Abh. Konigl. Preuss. Akad. Wissenschaften Jahre 1906,92, Berlin,1907, Stern-Katalog fur die Zone von -6 bis -10 Sudlicher Deklination fur das Aequinoktium 1890, erste und zweite Abteilung.
Auth.:	HERZ N.
Details on Acronym: HES2014
HES2014	(H.E.S.S. Collaboration+, 2014)
Write:	<<HES2014 N>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton observations of N=5 X-ray point sources in the field of HESS J1818-154.
Ref:	=2014A&A...562A..40H
by	HESS COLLABORATION , ABRAMOWSKI A., AHARONIAN F., AIT BENKHALI F., AKHPERJANIAN A.G., ANGUENER E., ANTON G., BALENDERAN S., BALZER A., BARNACKA A., BECHERINI Y., BECKER TJUS J., BERNLOEHR K., BIRSIN E., BISSALDI E., BITEAU J., BOETTCHER M., BOISSON C., BOLMONT J., BORDAS P., BRUCKER J., BRUN F., BRUN P., BULIK T., CARRIGAN S., CASANOVA S., CERRUTI M., CHADWICK P.M., CHALME-CALVET R., CHAVES R.C.G., CHEESEBROUGH A., CHRETIEN M., COLAFRANCESCO S., COLOGNA G., CONRAD J., COUTURIER C., CUI Y., DALTON M., DANIEL M.K., DAVIDS I.D., DEGRANGE B., DEIL C., DEWILT P., DICKINSON H.J., DJANNATI-ATAIE A., DOMAINKO W., DRURY L.O'C., DUBUS G., DUTSON K., DYKS J., DYRDA M., EDWARDS T., EGBERTS K., EGER P., ESPIGAT P., FARNIER C., FEGAN S., FEINSTEIN F., FERNANDES M.V., FERNANDEZ D., FIASSON A., FONTAINE G., FOERSTER A., FUESSLING M., GAJDUS M., GALLANT Y.A., GARRIGOUX T., GIAVITTO G., GIEBELS B., GLICENSTEIN J.F., GRONDIN M.-H., GRUDZINSKA M., HAEFFNER S., HAHN J., HARRIS J., HEINZELMANN G., HENRI G., HERMANN G., HERVET O., HILLERT A., HINTON J.A., HOFMANN W., HOFVERBERG P., HOLLER M., HORNS D., JACHOLKOWSKA A., JAHN C., JAMROZY M., JANIAK M., JANKOWSKY F., JUNG I., KASTENDIECK M.A., KATARZYNSKI K., KATZ U., KAUFMANN S., KHELIFI B., KIEFFER M., KLEPSER S., KLOCHKOV D., KLUZNIAK W., KNEISKE T., KOLITZUS D., KOMIN NU., KOSACK K., KRAKAU S., KRAYZEL F., KRUEGER P.P., LAFFON H., LAMANNA G., LEFAUCHEUR J., LEMIERE A., LEMOINE-GOUMARD M., LENAIN J.-P., LENNARZ D., LOHSE T., LOPATIN A., LU C.-C., MARANDON V., MARCOWITH A., MARX R., MAURIN G., MAXTED N., MAYER M., McCOMB T.J.L., MEHAULT J., MEINTJES P.J., MENZLER U., MEYER M., MODERSKI R., MOHAMED M., MOULIN E., MURACH T., NAUMANN C.L., DE NAUROIS M., NIEMIEC J., NOLAN S.J., OAKES L., OHM S., DE ONA WILHELMI E., OPITZ B., OSTROWSKI M., OYA I., PANTER M., PARSONS R.D., PAZ ARRIBAS M., PEKEUR N.W., PELLETIER G., PEREZ J., PETRUCCI P.-O., PEYAUD B., PITA S., POON H., PUEHLHOFER G., PUNCH M., QUIRRENBACH A., RAAB S., RAUE M., REIMER A., REIMER O., RENAUD M., DE LOS REYES R., RIEGER F., ROB L., ROMOLI C., ROSIER-LEES S., ROWELL G., RUDAK B., RULTEN C.B., SAHAKIAN V., SANCHEZ D.A., SANTANGELO A., SCHLICKEISER R., SCHUESSLER F., SCHULZ A., SCHWANKE U., SCHWARZBURG S., SCHWEMMER S., SOL H., SPENGLER G., SPIES F., STAWARZ L., STEENKAMP R., STEGMANN C., STINZING F., STYCZ K., SUSHCH I., SZOSTEK A., TAVERNET J.-P., TAVERNIER T., TAYLOR A.M., TERRIER R., TLUCZYKONT M., TRICHARD C., VALERIUS K., VAN ELDIK C., VAN SOELEN B., VASILEIADIS G., VENTER C., VIANA A., VINCENT P., VOELK H.J., VOLPE F., VORSTER M., VUILLAUME T., WAGNER S.J., WAGNER P., WARD M., WEIDINGER M., WEITZEL Q., WHITE R., WIERZCHOLSKA A., WILLMANN P., WOERNLEIN A., WOUTERS D., ZABALZA V., ZACHARIAS M., ZAJCZYK A., ZDZIARSKI A.A., ZECH A., ZECHLIN H.-S.
	Astron. Astrophys., 562A, 40-40 (2014)
	HESS J1818-154, a new composite supernova remnant discovered in TeV γ rays and X-rays.
o	Fig. 4, Table 1: <HES2014 N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HESS
HESS	(High Energy Stereoscopic System)
Write:	<<HESS JHHMM+DDdA>>
N:	about 50
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	Describes a major experiment in ground-based gamma-ray astronomy that started full scientific operation at the beginning of 2004. After initial confirmation of previously known or suspected sources it gradually observes more and more new sources and starts to detect previously unknown sources. 2005A&A...432L..25A, 2005Sci...307.1938A, first references with HESS objects.
Ref:	=2005A&A...432L..25A
by	AHARONIAN F. , AKHPERJANIAN A.G., AYE K.-M., BAZER-BACHI A.R., BEILICKE M., BENBOW W., BERGE D., BERGHAUS P., BERNLOEHR K., BOISSON C., BOLZ O., BORGMEIER C., BRAUN I., BREITLING F., BROWN A.M., BUSSONS GORDO J., CHADWICK P.M., CHOUNET L.-M., CORNILS R., COSTAMANTE L., DEGRANGE B., DJANNATI-ATAIE A., DRURY L.O'C., DUBUS G., ERGIN T., ESPIGAT P., FEINSTEIN F., FLEURY P., FONTAINE G., FUNK S., GALLANT Y.A., GIEBELS B., GILLESSEN S., GORET P., HADJICHRISTIDIS C., HAUSER M., HEINZELMANN G., HENRI G., HERMANN G., HINTON J.A., HOFMANN W., HOLLERAN M., HORNS D., DE JAGER O.C., JUNG I., KHELIFI B., KOMIN N., KONOPELKO A., LATHAM I.J., LE GALLOU R., LEMIERE A., LEMOINE M., LEROY N., LOHSE T., MARCOWITH A., MASTERSON C., McCOMB T.J.L., DE NAUROIS M., NOLAN S.J., NOUTSOS A., ORFORD K.J., OSBORNE J.L., OUCHRIF M., PANTER M., PELLETIER G., PITA S., PUEHLHOFER G., PUNCH M., RAUBENHEIMER B.C., RAUE M., RAUX J., RAYNER S.M., REDONDO I., REIMER A., REIMER O., RIPKEN J., ROB L., ROLLAND L., ROWELL G., SAHAKIAN V., SAUGE L., SCHLENKER S., SCHLICKEISER R., SCHUSTER C., SCHWANKE U., SIEWERT M., SOL H., STEENKAMP R., STEGMANN C., TAVERNET J.-P., TERRIER R., THEORET C.G., TLUCZYKONT M., VASILEIADIS G., VENTER C., VINCENT P., VISSER B., VOELK H.J., WAGNER S.J.
	Astron. Astrophys., 432, 25-29 (2005)
	Very high energy γ rays from the composite SNR G0.9+0.1.
o	text: <HESS JHHMM+DDd> N=2.
Ref:	=2005Sci...307.1938A
by	AHARONIAN F. , AKHPERJANIAN A.G., AYE K.-M., BAZER-BACHI A.R., BEILICKE M., BENBOW W., BERGE D., BERGHAUS P., BERNLOEHR K., BOISSON C., BOLZ O., BORGMEIER C., BRAUN I., BREITLING F., BROWN A.M., BUSSONS GORDO J., CHADWICK P.M., CHOUNET L.-M., CORNILS R., COSTAMANTE L., DEGRANGE B., DJANNATI-ATAIE A., DRURY L.O'C., DUBUS G., ERGIN T., ESPIGAT P., FEINSTEIN F., FLEURY P., FONTAINE G., FUNK S., GALLANT Y.A., GIEBELS B., GILLESSEN S., GORET P., HADJICHRISTIDIS C., HAUSER M., HEINZELMANN G., HENRI G., HERMANN G., HINTON J.A., HOFMANN W., HOLLERAN M., HORNS D., DE JAGER O.C., JUNG I., KHELIFI B., KOMIN N., KONOPELKO A., LATHAM I.J., LE GALLOU R., LEMIERE A., LEMOINE M., LEROY N., LOHSE T., MARCOWITH A., MASTERSON C., McCOMB T.J.L., DE NAUROIS M., NOLAN S.J., NOUTSOS A., ORFORD K.J., OSBORNE J.L., OUCHRIF M., PANTER M., PELLETIER G., PITA S., PUEHLHOFER G., PUNCH M., RAUBENHEIMER B.C., RAUE M., RAUX J., RAYNER S.M., REDONDO I., REIMER A., REIMER O., RIPKEN J., ROB L., ROLLAND L., ROWELL G., SAHAKIAN V., SAUGE L., SCHLENKER S., SCHLICKEISER R., SCHUSTER C., SCHWANKE U., SIEWERT M., SOL H., STEENKAMP R., STEGMANN C., TAVERNET J.-P., TERRIER R., THEORET C.G., TLUCZYKONT M., VAN DER WALT D.J., VASILEIADIS G., VENTER C., VINCENT P., VISSER B., VOELK H.J., WAGNER S.J.
	Science, 307, 1938-1942 (2005)
	A new population of very-high energy γ-ray sources in the Milky Way.
o	HESS J1303-63 = HESS J1303-631 in SIMBAD
o	Table 1, text: <HESS JHHMM+DDd> N=8 added.
Ref:	=2008A&A...481..401A
by	AHARONIAN F. , AKHPERJANIAN A.G., BAZER-BACHI A.R., BEHERA B., BEILICKE M., BENBOW W., BERGE D., BERNLOEHR K., BOISSON C., BOLZ O., BORREL V., BRAUN I., BRION E., BROWN A.M., BUEHLER R., BULIK T., BUESCHING I., BOUTELIER T., CARRIGAN S., CHADWICK P.M., CHOUNET L.-M., CLAPSON A.C., COIGNET G., CORNILS R., COSTAMANTE L., DEGRANGE B., DICKINSON H.J., DJANNATI-ATAIE A., DOMAINKO W., DRURY L.O'C., DUBUS G., DYKS J., EGBERTS K., EMMANOULOPOULOS D., ESPIGAT P., FARNIER C., FEINSTEIN F., FIASSON A., FOERSTER A., FONTAINE G., FUKUI Y., FUNK SEB., FUNK S., FUESSLING M., GALLANT Y.A., GIEBELS B., GLICENSTEIN J.F., GLUECK B., GORET P., HADJICHRISTIDIS C., HAUSER D., HAUSER M., HEINZELMANN G., HENRI G., HERMANN G., HINTON J.A., HOFFMANN A., HOFMANN W., HOLLERAN M., HOPPE S., HORNS D., JACHOLKOWSKA A., DE JAGER O.C., KENDZIORRA E., KERSCHHAGGL M., KHELIFI B., KOMIN N., KOSACK K., LAMANNA G., LATHAM I.J., LE GALLOU R., LEMIERE A., LEMOINE-GOUMARD M., LENAIN J.-P., LOHSE T., MARTIN J.M., MARTINEAU-HUYNH O., MARCOWITH A., MASTERSON C., MAURIN G., McCOMB T.J.L., MODERSKI R., MORIGUCHI Y., MOULIN E., DE NAUROIS M., NEDBAL D., NOLAN S.J., OLIVE J.-P., ORFORD K.J., OSBORNE J.L., OSTROWSKI M., PANTER M., PEDALETTI G., PELLETIER G., PETRUCCI P.-O., PITA S., PUEHLHOFER G., PUNCH M., RANCHON S., RAUBENHEIMER B.C., RAUE M., RAYNER S.M., REIMER O., RENAUD M., RIPKEN J., ROB L., ROLLAND L., ROSIER-LEES S., ROWELL G., RUDAK B., RUPPEL J., SAHAKIAN V., SANTANGELO A., SAUGE L., SCHLENKER S., SCHLICKEISER R., SCHROEDER R., SCHWANKE U., SCHWARZBURG S., SCHWEMMER S., SHALCHI A., SOL H., SPANGLER D., STAWARZ L., STEENKAMP R., STEGMANN C., SUPERINA G., TAKEUCHI T., TAM P.H., TAVERNET J.-P., TERRIER R., VAN ELDIK C., VASILEIADIS G., VENTER C., VIALLE J.P., VINCENT P., VIVIER M., VOELK H.J., VOLPE F., WAGNER S.J., WARD M.
	Astron. Astrophys., 481, 401-410 (2008)
	Discovery of very high energy γ-ray emission coincident with molecular clouds in the W 28 (G6.4-0.1) field.
o	Figs, Table 1: <HESS JHHMM+DDdA> (Nos J1800-240A to C). Paragr. 3.: <[AAB2008b] northeastern cloud>, <[AAB2008b] southern cloud>.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: HETDEX
HETDEX	(Hobby–Eberly Telescope Dark Energy Experiment)
Write:	<<HETDEX JHHMMSS.ss+DDMMSS.s>>
Object:	LAE + Poss. LAE (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	During three years of observations, the Hobby–Eberly Telescope Dark Energy Experiment (HETDEX) will collect data on at least one million galaxies that are 9 billion to 11 billion light-years away, yielding the largest map of the universe ever produced. For more information, visit: https://hetdex.org/hetdex.html Only the first references citing HETDEX sources are listed here.
Ref:	=2020ApJ...903...24M
by	MUKAE S. , OUCHI M., HILL G.J., GEBHARDT K., MENTUCH COOPER E., JEONG D., SAITO S., FABRICIUS M., GAWISER E., CIARDULLO R., FARROW D., DAVIS D., ZEIMANN G., FINKELSTEIN S.L., GRONWALL C., LIU C., ZHANG Y., BYROHL C., ONO Y., SCHNEIDER D.P., JARVIS M.J., CASEY C.M., MAWATARI K.
	Astrophys. J., 903, 24-24 (2020)
	Cosmological 3D H I gas map with HETDEX Lyα emitters and eBOSS QSOs at z = 2: IGM-Galaxy/QSO connection and a ~40 Mpc scale giant H II bubble candidate.
o	Tables 2-3: <HETDEX JHHMMSS.ss+DDMMSS.s> N=27+26. Fig. 13: <[MOH2020] EGS-QO1> N=1. Figs 13+16, Table 3: <[MOH2020] LAEN> (Nos LAE1-LAE4).
Ref:	=2021ApJ...920..122D
by	DAVIS D. , GEBHARDT K., MENTUCH COOPER E., CHISHOLM J., CIARDULLO R., FARROW D.J., FINKELSTEIN S.L., GRONWALL C., GAWISER E., HILL G.J., HOPP U., JEONG D., LANDRIAU M., LIU C., LUJAN NIEMEYER M., SCHNEIDER D.P., SNIGULA J., TUTTLE S.
	Astrophys. J., 920, 122-122 (2021)
	Detection of Lyman continuum from 3.0 < z < 3.5 galaxies in the HETDEX survey.
o	Table 1: <HETDEX JHHMMSS.ss+DDMMSS.s> N=214.
=E=	Catalogue in electronic form as <J/ApJ/903/24/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HETE
HETE	(High Energy Transient Explorer)
Write:	<<HETE Trigger NNNNN>> <<HETE JHHMM.m+DDMM>>
Object:	(Gamma) + X-ray binary (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Trigger number NNNNN of GRB and non-GRBs discovered by the HETE team. HETE triggers are found at http://gcn.gsfc.nasa.gov/hete_grbs.html X-ray burst sources discovered serendipitously by HETE have a format 'JHHMM.m+DDMM'.
Ref:	=2001GCN..1070....1R
by	RICKER G. , LAMB D., WOOSLEY S., VANDERSPEK R., CREW G., DOTY J., MONNELLY G., VILLASENOR J., BUTLER N., CLINE T., JERNIGAN J.G., LEVINE A., MARTEL F., MORGAN E., PIZZICHINI G., PRIGOZHIN G., KAWAI N., MATSUOKA M., SHIRASAKI Y., TAMAGAWA T., TORII K., SAKAMOTO T., YOSHIDA A., FENIMORE E., GALASSI M., GRAZIANI C., ATTEIA J.-L., BOER M., OLIVE J.-F., DEZALAY J.-P., HURLEY K.
	GRB Coordinates Network, Circular Service, 1070, 1-None (2001)
	SGR1806-20: A Second, Intense Burst Localized by HETE.
o	<HETE Trigger NNNNN> N=1.
Ref:	=2005ATel..516....1V
by	VANDERSPEK R. , MORGAN E., CREW G., GRAZIANI C., SUZUKI M.
	The Astronomer's Telegram, 516, 1-None (2005)
	Possible new X-ray burst source detected by HETE.
o	<HETE JHHMM.m+DDMM> N=1.
Ref:	=2005ApJ...629..311S
by	SAKAMOTO T. , LAMB D.Q., KAWAI N., YOSHIDA A., GRAZIANI C., FENIMORE E.E., DONAGHY T.Q., MATSUOKA M., SUZUKI M., RICKER G., ATTEIA J.-L., SHIRASAKI Y., TAMAGAWA T., TORII K., GALASSI M., DOTY J., VANDERSPEK R., CREW G.B., VILLASENOR J., BUTLER N., PRIGOZHIN G., JERNIGAN J.G., BARRAUD C., BOER M., DEZALAY J.-P., OLIVE J.-F., HURLEY K., LEVINE A., MONNELLY G., MARTEL F., MORGAN E., WOOSLEY S.E., CLINE T., BRAGA J., MANCHANDA R., PIZZICHINI G., TAKAGISHI K., YAMAUCHI M.
	Astrophys. J., 629, 311-327 (2005)
	Global characteristics of X-ray flashes and X-Ray-Rich γ-ray bursts observed by HETE-2.
o	Table 1: <HETE Trigger NNNNN> N=45.
=E=	Catalogue in electronic form as J/other/GCN/1070.1
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Hetzler
Hetzler	(Hetzler)
Write:	<<Hetzler R NNa>>
N:	96
Object:	(IR) * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 4: infrared stars in 8 fields (Nos I-VIII), N=24+7+3+10+19+2+17+15
Ref:	=1937ApJ....86..509H
by	HETZLER C.
	Astrophys. J., 86, 509-528 (1937)
	Infrared stellar surveys and index sequences.
o	Tables 4: <Hetzler R NNa> N=96.
Origin	of the Acronym: L (1965ApJ...142.1249J)
Details on Acronym: [HEV2001]
[HEV2001]	(Hunter+Elmegreen+Van Woerden, 2001)
Write:	<<[HEV2001] NN>>
N:	20
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=20 VLA radio-sources in NGC 2366.
in source:	NGC 2366
Ref:	=2001ApJ...556..773H
by	HUNTER D.A. , ELMEGREEN B.G., VAN WOERDEN H.
	Astrophys. J., 556, 773-800 (2001)
	Neutral hydrogen and star formation in the irregular galaxy NGC 2366.
o	Table 1, Fig.2: <[HEV2001] NN> (Nos 1-20).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Hewett
Hewett	(Hewett+)
Write:	<<Hewett N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Discovey of a new PN at the proximity of PG 1034+001 n the SDSS, he largest in the sky.
Ref:	=2003ApJ...599L..37H
by	HEWETT P.C. , IRWIN M.J., SKILLMAN E.D., FOLTZ C.B., WILLIS J.P., WARREN S.J., WALTON N.A.
	Astrophys. J., 599, 37-40 (2003)
	Serendipity and the Sloan Digital Sky Survey: discovery of the largest known planetary nebula on the sky.
o	<Hewett N> (No. 1).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Hf
Hf	(Hoffleit)
*****	Avoid the usage of Hf, prefer [H53]
Origin	of the Acronym: L (2000A&A...357..308G)
Details on Acronym: Hf
Hf	(Hoffleit)= (H) = (Hoffleit)
Write:	<<PN Hf NN>> <<PN Hf 2-N>>
N:	6+2
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Among the 63 nebulae [H53], 6 objects are PN (Nos 4, 38, 39, 48, 62, 69). In 1967PK....C......1P, 2 other 'Hf' PN are designated with a format '2-N' (Nos 2-1 and 2-2).
Ref:	=1953AnHar.119...37H
by	HOFFLEIT D.
	Ann. Astron. Obs. Harvard Coll., 119, 37-None (1953)
	A preliminary survey of nebulosities and associated B-stars in Car.
o	Catalogue: <[H53] NN> (Nos 1-69) among which: <PN Hf NN> N=6 (Nos 4, 38, 39, 48, 62, 69).
Details on Acronym: [HF2008]
[HF2008]	(Hammell+Fesen, 2008) (Not yet in Simbad)
Write:	<<[HF2008] NNNN>>
N:	1825
Object:	Ejecta Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST images of Cas A SNR to identify high-velocity knots of ejecta ouside the SNR.
in source:	NAME Cas A
Ref:	=2008ApJS..179..195H
by	HAMMELL M.C. , FESEN R.A.
	Astrophys. J., Suppl. Ser., 179, 195-208 (2008)
	A catalog of outer ejecta knots in the Cassiopeia A supernova remnant.
o	Table 2: <[HF2008] NNNN> (Nos 1-1825).
=E=	Catalogue in electronic form as J/ApJS/179/195
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HF96]
[HF96]	(Hurford+Fesen, 1996)= (FMK)
Write:	<<[HF96] FMK N>>
N:	5
Object:	Knot (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=5 Fast-Moving Knots, format 'FMK N', (Nos 1-5). and N=2 Quasi Stationary Flocculi, 'KB QSF R2'and 'R10' See also [GF2001].
in source:	NAME Cas A
Ref:	=1996ApJ...469..246H
by	HURFORD A.P. , FESEN R.A.
	Astrophys. J., 469, 246-254 (1996)
	Reddening measurements and physical conditions for Cassiopeia A from optical and near-infrared spectra.
o	Filament 1 = [BM54] Cas 1, R2 and R10 = KB QSF R2 and R10, p.250: 1Q1 = [KC77] 1Q1, p.252: KB 33 = KB MK 33
o	Table 1: <[HF96] FMK N> (Nos 1-5)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HFB2000]
[HFB2000]	(Huggins+Forveille+Bachiller+, 2000) (Not yet in Simbad)
Write:	<<[HFB2000] A>>
N:	3
Object:	Outflow (SIMBAD class: PartofCloud = Part of Cloud)
Note:	(Nos A-C), 3 outflows from PN M 1-16.
in source:	PN M 1-16
Ref:	=2000ApJ...544..889H
by	HUGGINS P.J. , FORVEILLE T., BACHILLER R., COX P.
	Astrophys. J., 544, 889-894 (2000)
	The shaping of planetary nebulae by bipolar outflows: the case of M1-16.
o	Fig.1: <[HFB2000] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HFB2002]
[HFB2002]	(Harris+Finoguenov+Hardcastle+, 2002) (Not yet in Simbad)
Write:	<<[HFB2002] NN.N>>
N:	2
Object:	Knot (SIMBAD class: X = X-ray Source)
Note:	N=2 X-ray emission knots in the jet of M 84. The designation is accordig to their angular distance from the core in arcseconds.
in source:	M 84 = NGC 4374
Ref:	=2002ApJ...580..110H
by	HARRIS D.E. , FINOGUENOV A., BRIDLE A.H., HARDCASTLE M.J., LAING R.A.
	Astrophys. J., 580, 110-113 (2002)
	X-ray detection of the inner jet in the radio galaxy M84.
o	p. 113 : Knots D and HST-1 in M87 are [DAF68] D and [PBZ99] HST-1
o	<[HFB2002] AN.N> (Nos N2.5, N3.3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HFB2009]
[HFB2009]	(Huxor+Ferguson+Barker+, 2009) (Not yet in Simbad)
Write:	<<[HFB2009] HM33-A>>
N:	5
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	Discovery of N=5 globular clusters in M33, using INT/WFC (La Palma) observations and HST/ACS data.
in source:	M 33 = NGC 598
Ref:	=2009ApJ...698L..77H
by	HUXOR A. , FERGUSON A.M.N., BARKER M.K., TANVIR N.R., IRWIN M.J., CHAPMAN S.C., IBATA R., LEWIS G.
	Astrophys. J., 698L, 77-81 (2009)
	The discovery of remote globular clusters in M33.
o	Table 1, Fig. 2: <[HFB2009] HM33-A> (Nos A-D).
Ref:	=2011ApJ...730..112C
by	COCKCROFT R. , HARRIS W.E., FERGUSON A.M.N., HUXOR A., IBATA R., IRWIN M.J., McCONNACHIE A.W., WOODLEY K.A., CHAPMAN S.C., LEWIS G.F., PUZIA T.H.
	Astrophys. J., 730, 112 (2011)
	The M33 globular cluster system with PAndAS data: the last outer halo cluster?
o	Fig. 1, Tables 3-4: <[HFB2009] HM33-A> (No. E) added, <[CHF2011] M33 S> N=1.
o	Cluster S is [SVA2008] M 33-EC1 in SIMBAD.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HFC93]
[HFC93]	(Hui+Ford+Ciardullo+, 1993)
Write:	<<[HFC93] NNNNN>>
N:	785
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	N=785 among (Nos 1-42136)
in source:	Cen A = NGC 5128
Ref:	=1993ApJS...88..423H
by	HUI X. , FORD H.C., CIARDULLO R., JACOBY G.H.
	Astrophys. J., Suppl. Ser., 88, 423-431 (1993)
	The planetary nebula system and dynamics of NGC 5128. II. A planetary nebula catalog.
o	Tables 2, 3: not in Simbad.
o	Table 1: <[HFC93] NNNNN> N=785 among 42136
=E=	Catalogue in electronic form as J/ApJS/88/423
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HFD2003]
[HFD2003]	(Hornoch+Fiaschi+Di Mille+, 2003)
Write:	<<[HFD2003] JHHMMSS.ss+DDMMSS.s>>
N:	3+2
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Stat:	is completely incorporated in Simbad
Note:	Lelekovice and Astronomical Observatory G. Colombo observations. Discovery of three then two new novae in M 31.
in source:	M 31 = NGC 224
Ref:	=2003IAUC.8165....2H
by	HORNOCH K. , FIASCHI M., DI MILLE F., TIVERON D., SAROUNOVA L.
	IAU Circ., 8165, 2-None (2003)
	Novae in M31.
o	<[HFD2003] JHHMMSS.ss+DDMMSS.s> N=3.
Ref:	=2003IAUC.8222....2H
by	HORNOCH K. , FIASCHI M., DI MILLE F., TIVERON D.
	IAU Circ., 8222, 2-None (2003)
	Novae in M31.
o	<[HFD2003] JHHMMSS.ss+DDMMSS.s> N=2 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HFD2019]
[HFD2019]	(Hyman+Frail+Deneva+, 2019)
Write:	<<[HFD2019] CJHHMM+DDMM>> <<[HFD2019] CHHMM+DDMM>> (not recognised by Simbad, but found in literature)
N:	7
Object:	Poss. Psr (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA observations of N=7 pulsar candidates toward the Galactic Center.
Ref:	=2019ApJ...876...20H
by	HYMAN S.D. , FRAIL D.A., DENEVA J.S., KASSIM N.E., McLAUGHLIN M.A., KOOI J.E., RAY P.S., POLISENSKY E.J.
	Astrophys. J., 876, 20-20 (2019)
	A search for pulsars in steep-spectrum radio sources toward the Galactic Center.
o	Tables 1+3+4: <[HFD2019] CJHHMM+DDMM> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HFE
HFE	(Hoffmann+Frederick+Emery)= (Hoff)
Write:	<<HFE NN>>
N:	72
Object:	(Far IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Ref:	=1971ApJ...170L..89H
by	HOFFMANN W.F. , FREDERICK C.L., EMERY R.J.
	Astrophys. J., 170, 89-97 (1971)
	100-micron survey of the galactic plane.
o	Table 3: <HFE NN> (Nos 1-72)
=E=	Catalogue in electronic form as <II/56/>
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HFE2003]
[HFE2003]	(Humphrey+Fabbiano+Elvis+, 2003)
Write:	<<[HFE2003] NGC NNNN PSX-NN>> <<[HFE2003] IZW18 PSX-N>> <<[HFE2003] IC 2574 PSX-NN>> <<[HFE2003] NGC NNNN ESX-N>>
N:	61+10
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Search for Ultraluminous X-ray sources in 11 galaxies with Chandra. In the format 'PSX' stands for Point sources, 'ESX' for Extended sources.
in source:	NGC 1132
in source:	NGC 1399
in source:	NGC 1291
in source:	NGC 2681
in source:	NGC 253
in source:	NGC 4631
in source:	NGC 4636
in source:	NGC 4697
in source:	NGC 3184
in source:	ZW I 18 = Mrk 116
in source:	IC 2574
Ref:	=2003MNRAS.344..134H
by	HUMPHREY P.J. , FABBIANO G., ELVIS M., CHURCH M.J., BALUCINSKA-CHURCH M.
	Mon. Not. R. Astron. Soc., 344, 134-148 (2003)
	Ultraluminous X-ray source populations in normal galaxies: a preliminary survey with Chandra.
o	Table 4: <[HFE2003] NGC NNNN PSX-NN> N=59, <[HFE2003] IZW18 PSX-N> No. 1), <[HFE2003] IC 2574 PSX-N> (No. 1). Table 5: <[HFE2003] NGC NNNN ESX-NN> N=10.
=E=	Catalogue in electronic form as J/MNRAS/344/134
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HFE2012]
[HFE2012]	(Han+Frenck+Eke+, 2012)
Write:	<<[HFE2012] AN>>
N:	5
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Use of 45 months of Fermi LAT data. N=5 point sources (sources in Virgo and Fornax are prefixed V and F in their names, respectively).
in source:	NAME Virgo Cluster
in source:	NAME Fornax Cluster
Ref:	=2012MNRAS.427.1651H
by	HAN J. , FRENK C.S., EKE V.R., GAO L., WHITE S.D.M., BOYARSKY A., MALYSHEV D., RUCHAYSKIY O.
	Mon. Not. R. Astron. Soc., 427, 1651-1665 (2012)
	Constraining extended γ-ray emission from galaxy clusters.
o	Table A1: <[HFE2012] AN> (Nos V1-V4, F1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HFE83]
[HFE83]	(Helmer+Fabricius+Einicke+, 1983)
Write:	<<[HFE83] NNNN>>
N:	1572
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1983A&AS...53..223H
by	HELMER L. , FABRICIUS C., EINICKE O.H., THOBURN C.
	Astron. Astrophys., Suppl. Ser., 53, 223-245 (1983)
	Meridian observations made with the Carlsberg automatic meridian circle at Brorfelde (Copenhagen University Observatory) 1981-1982.
o	<[HFE83] NNNN> N=1577
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HFF
HFF	(Hubble Flanking Field)
*****	Avoid the usage of HFF, prefer [FKR97]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HFF
HFF	(Hubble Frontier Fields SN)
Write:	<<HFF YYAaa>>
Object:	Poss. SN (SIMBAD class: Supernova_Candidate = SuperNova Candidate)
Note:	HST observations of supernova candidates, as part of the Hubble Frontier Fields (HFF) program.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HFF-DS
HFF-DS	(Hubble Frontier Fields - DeepSpace) (Not yet in Simbad)
*****	Avoid the usage of HFF-DS, prefer [SLM2018]
Origin	of the Acronym: L (2023ApJ...942L..25M)
Details on Acronym: HFG
HFG	(Heckathorn+Fesen+Gull)= (HeFe)
Write:	<<PN HFG N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	HFG 1 = PN G136.3+05.5 = PK 136+05 1
Ref:	=1982A&A...114..414H
by	HECKATHORN J.N. , FESEN R.A., GULL T.R.
	Astron. Astrophys., 114, 414-418 (1982)
	Discovery of a large, high-excitation planetary nebula at l=136, b=+5.
Details on Acronym: [HFG2013]
[HFG2013]	(Harvey+Fallscheer+Ginsburg+, 2013)
Write:	<<[HFG2013] NN>> <<[HFG2013] CSO NN>>
N:	60+18
Object:	(FIR) + (mm) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Herschel (PACS and SPIRE) observations of N=60 compact sources and CSO Bolocam 1.1mm observations of N=18 cold, compact sources.
in source:	NAME Auriga-California Molecular Cloud
Ref:	=2013ApJ...764..133H
by	HARVEY P.M. , FALLSCHEER C., GINSBURG A., TEREBEY S., ANDRE P., BOURKE T.L., DI FRANCESCO J., KONYVES V., MATTHEWS B.C., PETERSON D.E.
	Astrophys. J., 764, 133 (2013)
	A first look at the Auriga-California giant molecular cloud with Herschel and the CSO: census of the young stellar objects and the dense gas.
o	Table 2: <[HFG2013] NN> (Nos 1-60). Table 3: <[HFG2013] CSO NN> (Nos 1-18).
=E=	Catalogue in electronic form as J/ApJ/764/133
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HFH2015]
[HFH2015]	(Hackstein+Fein+Haas+, 2015)= (GDS) (Not yet in Simbad)
Write:	<<[HFH2015] GDS JHHMMSSs+DDMMSS>> <<[HFH2015] GDS_JHHMMSSs+DDMMSS>> (not recognised by Simbad, but found in literature)
N:	64151
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	First complete version of the southern Galactic Disk Survey (GDS) performed at the Universitätssternwarte Bochum near Cerro Armazones in Chile. Catalog of N=64151 variable sources. See also [HHR2012].
Ref:	=2015AN....336..590H
by	HACKSTEIN M. , FEIN C., HAAS M., RAMOLLA M., POZO NUNEZ F., BARR DOMINGUEZ A., KADERHANDT L., THOMSCH K., NIEDWOROK N., WESTHUES C., CHINI R.
	AN, 336, 590 (2015)
	The Bochum Survey of the Southern Galactic Disk: II. Follow-up measurements and multi-filter photometry for 1323 square ° monitored in 2010-2015.
o	<[HFH2015] GDS JHHMMSSs+DDMMSS> N=64151.
=E=	Catalogue in electronic form as <J/AN/336/590/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HFI2009]
[HFI2009]	(Holden+Franx+Illingworth+, 2009)= (GAL)
Write:	<<[HFI2009] JHHMMSS.ss+DDMMSS.s>> <<[HFI2009] GAL HHMMSS.ss+DDMMSS.s>> (not recognised by Simbad, but found in literature)
N:	60
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck II DEIMOS observations of Cl 1226+33.
in source:	ClG J1226+3332
Ref:	=2009ApJ...693..617H
by	HOLDEN B.P. , FRANX M., ILLINGWORTH G.D., POSTMAN M., VAN DER WEL A., KELSON D.D., BLAKESLEE J.P., FORD H., DEMARCO R., MEI S.
	Astrophys. J., 693, 617-633 (2009)
	The ellipticities of cluster early-type galaxies from z ~ 1 to z ~ 0: no evolution in the overall distribution of bulge-to-disk ratios.
o	Table 4: <[HFI2009] JHHMMSS.ss+DDMMSS.s> N=60.
=E=	Catalogue in electronic form as <J/ApJ/693/617/>
Details on Acronym: [HFK2000]
[HFK2000]	(Hoekstra+Franx+Kuiken, 2000)
Write:	<<[HFK2000] W>>
N:	3
Object:	Clump (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations. N=3 clumps in the mass distribution of ClG 1054-0321 (1E 1054.4-0321). See also [DVG98], [NA2000], [JCB2001], [JWF2005].
in source:	1E 1054.4-0321 = ClG 1054-0321
Ref:	=2000ApJ...532...88H
by	HOEKSTRA H. , FRANX M., KUIJKEN K.
	Astrophys. J., 532, 88-108 (2000)
	Hubble space telescope weak-lensing study of the z=0.83 cluster MS 1054-03.
o	Table 4: <[HFK2000] W> (Nos E, C, W).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HFK95]
[HFK95]	(Hambly+Fitzsimmons+Keenan+, 1995)
Write:	<<[HFK95] NNNN-NNNN>>
N:	9
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=9 stellar-like objects in the halo of M 31.
in source:	M 31 = NGC 224
Ref:	=1995ApJ...448..628H
by	HAMBLY N.C. , FITZSIMMONS A., KEENAN F.P., DUFTON P.L., BROWN P.J.F., IRWIN M.J., ROLLESTON W.R.J.
	Astrophys. J., 448, 628-633 (1995)
	A photometric and spectroscopic survey for young stars in the halo of M31.
o	Table 1: <[HFK95] NNNN-NNNN> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HFP
HFP	(High Frequency Peaker)
*****	Avoid the usage of HFP, prefer [ODS2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HFP2000]
[HFP2000]	(Haberl+Filipovic+Pietsch+, 2000)= (RP) = (HFPK00)
Write:	<<[HFP2000] NNN>>
N:	517
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Sample of variable X-ray sources observed by ROSAT PSPC in the SMC. See also ROSAT PSPC [HP99] in the LMC. See also ROSAT HRI in the LMC and SMC: [SHP2000].
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2000A&AS..142...41H
by	HABERL F. , FILIPOVIC M.D., PIETSCH W., KAHABKA P.
	Astron. Astrophys., Suppl. Ser., 142, 41-57 (2000)
	A ROSAT PSPC catalogue of X-ray sources in the SMC region.
o	[HFP186] opt. id not confirmed (O7III in KPF1999); see also 2003ApJ.586 .983N p. 991
o	Table 2: <[HFP2000] NNN> N=517 among (Nos 8-737).
=E=	Catalogue in electronic form as J/A+AS/142/41
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HFPK00
HFPK00	(Haberl+Filipovic+Pietsch+Kahabka, 2000)
*****	Avoid the usage of HFPK00, prefer [HFP2000]
Origin	of the Acronym: L (2000A&AS..147...75S)
Details on Acronym: [HFR2007]
[HFR2007]	(Hatchell+Fuller+RIcher+, 2007)
Write:	<<[HFR2007] NNN>> <<[HFR2007] clf NN>>
N:	81+6
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	SCUBA observations of the Perseus molecular cloud. See also [HRF2005].
in source:	NAME Perseus Molecular Cloud
Ref:	=2007A&A...468.1009H
by	HATCHELL J. , FULLER G.A., RICHER J.S., HARRIES T.J., LADD E.F.
	Astron. Astrophys., 468, 1009-1024 (2007)
	Star formation in Perseus. II. SEDs, classification, and lifetimes.
o	Tables 4, 5: <[HFR2007] NNN> N=81 among (Nos 1-101), <[HFR2007] clf NN> N=6 among (Nos 55-79).
=E=	Catalogue in electronic form as J/A+A/468/1009
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HFR97]
[HFR97]	(Holland+Fahlman+Richer, 1997) (Not yet in Simbad)
Write:	<<[HFR97] G302 WFN NNNN>> <<[HFR97] G312 WFN NNNN>>
N:	12289+3355
Object:	* in Cl* (SIMBAD class: Star)
Note:	HST WFPC2 observations. Table 3: * in G302 (= SKHB 302), format 'G302 WFN NNNN'. Table 4: * in G312 (= SKHB 312), format 'G312 WFN NNNN'. In the format, 'WFN' (WF2, WF3, WF4) is the CCD the star was observed on.
in source:	M 31:SKHB 302 = SKHB 302
in source:	M 31:SKHB 312 = SKHB 312
Ref:	=1997AJ....114.1488H
by	HOLLAND S. , FAHLMAN G.G., RICHER H.B.
	Astron. J., 114, 1488-1507 (1997)
	Deep HST V- and I-band observations of two globular clusters in the halo of M31.
o	Objects in tables 3, 4 are not in SIMBAD
o	Table 3: <[HFR97] G302 WFN NNNN> N=12289. Table 4: <[HFR97] G312 WFN NNNN> N=3355.
=E=	Catalogue in electronic form as J/AJ/114/1488
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HFS
HFS	(Haro, Flare Star)
*****	Avoid the usage of HFS, prefer [HC73]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: HFS
HFS	(Haro, Flare Star)
*****	Avoid the usage of HFS, prefer [HC74]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: HFS1
HFS1	(Haro, Flare *, table 1)
*****	Avoid the usage of HFS1, prefer HPRA
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [HFS2015]
[HFS2015]	(Hayes+Friel+Slack+, 2015)
Write:	<<[HFS2015] NNNN>>
N:	6294
Object:	* (SIMBAD class: Star)
Note:	WIYN 0.9m telescope S2KB photometric and WIYN 3.5m telescope spectroscopic observations of N=6294 stars of the old open cluster Czernik 30.
in source:	Cl Czernik 30
Ref:	=2015AJ....150..200H
by	HAYES C.R. , FRIEL E.D., SLACK T.J., BOBERG O.M.
	Astron. J., 150, 200 (2015)
	Properties of the old open cluster Czernik 30.
o	Table 3: <[HFS2015] NNNN> (Nos 1-6294).
=E=	Catalogue in electronic form as J/AJ/150/200
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HFS4
HFS4	(Haro, Flare , table 4)= (Ton) (Not yet in Simbad)*
Write:	<<HFS4 NN>>
N:	11
Object:	Flare * (SIMBAD class: Eruptive* = Eruptive Variable)
in source:	NAME TMC
Ref:	=1968SSS.....7..141H
by	HARO G.
	Stars and stellar systems., 7, 141-None (1968)
	Flare stars.
o	Nebulae and interstellar matter, 1968, Ed. Middlehurst B.M., Serie Stars and stellar systems, vol. 7, p. 141.
o	Table 1: <HPRA NNN> (Nos 1-176). Table 4: <HFS4 NN> (Nos 1-11).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [HFS92]
[HFS92]	(Holtzman+Faber+Shaya+, 1992)= (H)
Write:	<<[HFS92] NN>> <<[HFS92] NNN>>
N:	64
Object:	Blue Obj. (SIMBAD class: blue = Blue Object)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-58) with someones missing, for objects on chip 6. Format 'NNN' (always 3 digits) for objects on other chips, with the chip given by the first digit.
in source:	NGC 1275 = 3C 84
Ref:	=1992AJ....103..691H
by	HOLTZMAN J.A. , FABER S.M., SHAYA E.J., LAUER T.R., GROTH E.J., HUNTER D.A., BAUM W.A., EWALD S.P., HESTER J.F., LIGHT R.M., LYNDS C.R., O'NEIL E.J.Jr, WESTPHAL J.A.
	Astron. J., 103, 691-702 (1992)
	Planetary camera observations of NGC 1275: discovery of a central population of compact massive blue star clusters.
o	<[HFS92] NN> (Nos 1-58) and <[HFS92] NNN> always 3 digits N=8
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HFS97]
[HFS97]	(Hasinger+Fischer+Schwope+, 1997)
Write:	<<[HFS97] N>>
N:	4
Object:	G (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=4 interacting galaxies, observed in ROSAT All-Sky Survey. No. 1 = RHS 97 = VV 697, an interacting Seyfert galaxy.
Ref:	=1997AN....318..329H
by	HASINGER G. , FISCHER J.-U., SCHWOPE A.D., BOLLER T., TRUMPER J., VOGES W.
	Astron. Nachr., 318, 329-334 (1997)
	Interacting galaxies. The X-ray view.
o	RHS 66 from RHS survey.
o	Fig.3: <[HFS97] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HFS98]
[HFS98]	(Hill+Fanelli+Smith+, 1998)
Write:	<<[HFS98] Region N>> <<[HFS98] Source NN>>
N:	4+57
Object:	Region + (UV) (SIMBAD class: UV = UV-emission Source)
Note:	Observations of NGC 4449 with the UIT aboard Astro 2 Space Shuttle mission. Table 3: N=4 Froth regions. Tables 7, 8: N=57 (UV) sources. See also [HHS94].
in source:	NGC 4449
Ref:	=1998ApJ...507..179H
by	HILL R.S. , FANELLI M.N., SMITH D.A., BOHLIN R.C., NEFF S.G., O'CONNELL R.W., ROBERTS M.S., SMITH A.M., STECHER T.P.
	Astrophys. J., 507, 179-198 (1998)
	Ultraviolet imaging of the irregular galaxy NGC 4449 with the ultraviolet imaging telescope: photometry and recent star formation history.
o	Table 3: <[HFS98] Region N> (Nos 1-4). Tables 7, 8: <[HFS98] Source NN> (Nos 1-57).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HFT2009]
[HFT2009]	(Healey+Fuhrmann+Taylor+, 2009)
Write:	<<[HFT2009] JHHMM+DDMM>> <<[HFT2009] JHHMMSS.sss+DDMMSS.ss>>
N:	368+156
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Effelsberg 4.85GHz observations of N=368 sources and VLA 8.44GHz follow-up observations of N=156 sources towards the North polar cap and the "PMN holes". Use of NVSS data.
Ref:	=2009AJ....138.1032H
by	HEALEY S.E. , FUHRMANN L., TAYLOR G.B., ROMANI R.W., READHEAD A.C.S.
	Astron. J., 138, 1032-1036 (2009)
	Filling in the gaps in the 4.85 GHz sky.
o	Tables 1-2: <[HFT2009] JHHMM+DDMM> N=368, <[HFT2009] JHHMMSS.sss+DDMMSS.ss> N=156.
=E=	Catalogue in electronic form as <J/AJ/138/1032/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HFT78]
[HFT78]	(Harten+Felli+Tofani, 1978) (Not yet in Simbad)
Write:	<<[HFT78] NN>> <<[HFT78] Shell A>> <<[HFT78] Ridge>>
N:	19+2+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Radio emission study of Sh 2-132. Map in Fig.1: N=19 small diameter sources, 2 shells and 1 ridge.
in source:	SH 2-132
Ref:	=1978A&A....70..205H
by	HARTEN R.H. , FELLI M., TOFANI G.
	Astron. Astrophys., 70, 205-211 (1978)
	A study of the radio continuum emission of the giant H II region S 132.
o	Table 2: <[HFT78] NN> (Nos 1-19). Table 3: <[HFT78] Shell A> (Nos A-B), <[HFT78] Ridge> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HFV2013]
[HFV2013]	(Huxor+Ferguson+Veljanoski+, 2013)
Write:	<<[HFV2013] SCN>>
N:	3
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	N=3 globular clusters in NGC 6822. Use of archival CFHT MegaCam data. The notation used here is a continuation of the naming convention used by Hwang et al. (2011ApJ...738...58H): see also [HLL2011].
in source:	NGC 6822
Ref:	=2013MNRAS.429.1039H
by	HUXOR A.P. , FERGUSON A.M.N., VELJANOSKI J., MacKEY A.D., TANVIR N.R.
	Mon. Not. R. Astron. Soc., 429, 1039-1044 (2013)
	Three newly discovered globular clusters in NGC 6822.
o	Fig. 1, Tables 1-2: <[HFV2013] SCN> (Nos SC5-SC7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HG
HG	(Hyades, Giclas)= (G) = (GH)
Write:	<<HG 7-NNN>> <<HG 8-NN>>
N:	292
Object:	WD (SIMBAD class: WhiteDwarf = White Dwarf)
Rem:	WD Nomenclature.
in source:	NAME Hyades
Ref:	=1962LowOB...5..257G
by	GICLAS H.L. , BURNHAM R.Jr, THOMAS N.G.
	Lowell Obs. Bull., 5, 257-280 (1962)
	A proper motion survey in the Hyades.
o	Table I: <HG 7-NNN> (Nos 7-1 to 7-259). Table IV: <HG 8-NN> (Nos 8-1 to 8-82)
Details on Acronym: HG
HG	(Huchra+Geller)
*****	Avoid the usage of HG, prefer [HG82]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HG
HG	(Harvey+Gatley)
*****	Avoid the usage of HG, prefer [HG83]
Origin	of the Acronym: L (1987ApJ...317..173H)
Details on Acronym: HG
HG	(Hunter+Gallagher)
*****	Avoid the usage of HG, prefer [HG85]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HG82]
[HG82]	(Huchra+Geller, 1982)= (GNO) = (HG) = (HGCG) = (NB)
Write:	<<[HG82] NN>>
N:	92
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Ref:	=1982ApJ...257..423H
by	HUCHRA J.P. , GELLER M.J.
	Astrophys. J., 257, 423-437 (1982)
	Groups of Galaxies. I. Nearby groups.
o	Tables 3, 5: <[HG82] NN> N=92
=E=	Catalogue in electronic form as VII/86
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HG83]
[HG83]	(Harvey+Gatley, 1983)= (HG) = ([HG83a]) = (IRS)
Write:	<<[HG83] IRS-I-NWW>> <<[HG83] IRS-IV-N>> <<[HG83] IRS-V-NW>>
N:	6+8+10
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	IR sources in MFSW I, format 'IRS-I-NWW': (Nos 1-4, 1E, 1W, 1SE, 1SW) IR sources in MFSW IV, format 'IRS-IV-N': (Nos 1-6) IR sources in MFSW V, format 'IRS-V-NW': (Nos 1-8, 4E, 4W). See also [SDW85] and KDJ
in source:	NGC 6334:MFSW I = MFSW I
in source:	NGC 6334:MFSW IV = MFSW IV
in source:	NGC 6334:MFSW V = MFSW V
Ref:	=1983ApJ...269..613H
by	HARVEY P.M. , GATLEY I.
	Astrophys. J., 269, 613-624 (1983)
	Infrared observations of OB star formation in NGC 6334.
o	Table 1, col. (4), and Table 4: <[HG83] IRS-I-N> (Nos 1-4). Table 5: <[HG83] IRS-IV-N> (Nos 1-6). Table 6: <[HG83] IRS-V-N> (Nos 1-6)
Ref:	=1984ApJ...280L..19H
by	HARVEY P.M. , WILKING B.A.
	Astrophys. J., 280, 19-22 (1984)
	NGC 6334-V - an infrared bipolar nebula.
o	Table 1: <[HG83] IRS-V-NW> (Nos 7-8, 4E, 4W) added
Ref:	=1996A&A...307..591P
by	PERSI P. , ROTH M., TAPIA M., MARENZI A.R., FELLI M., TESTI L., FERRARI-TONIOLO M.
	Astron. Astrophys., 307, 591-598 (1996)
	Shocked molecular hydrogen emission in the bipolar outflow NGC 6334 I.
o	Table 1: <[HG83] IRS-I-NWW> (Nos 1E, 1W, 1SE, 1SW)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HG83a]
[HG83a]	(Harvey+Gatley, 1983)
*****	Avoid the usage of [HG83a], prefer [HG83]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HG83b]
[HG83b]	(Hertz+Grindlay, 1983)
Write:	<<[HG83b] NGC 5139 A>> <<[HG83b] NGC 6656 A>>
N:	5+4
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Einstein IPC observations of NGC 5139 and NGC 6656.
in source:	NGC 5139 = ome Cen
in source:	M 22 = NGC 6656
Ref:	=1983ApJ...275..105H
by	HERTZ P. , GRINDLAY J.E.
	Astrophys. J., 275, 105-119 (1983)
	An X-ray survey of globular clusters and their X-ray luminosity function.
o	Tables 6, 9: <[HG83b] NGC 5139 A> (Nos A-E), <[HG83b] NGC 6656 A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HG85]
[HG85]	(Hunter+Gallagher, 1985)= (HG)
Write:	<<[HG85] DDO NNN NN>> <<[HG85] DDO 49 cen>> <<[HG85] IC 10 N>>
N:	74
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Tables 5, 6, 7: HII in 14 'DDO' galaxies, and in 'IC 10' galaxy. HII regions in IC 1613, M 33, DDO 209, and in table 8 are not [HG85] regions.
in source:	DDO 11
in source:	DDO 26
in source:	DDO 47
in source:	DDO 49
in source:	DDO 50 = Holmberg II
in source:	DDO 53
in source:	DDO 64
in source:	DDO 68
in source:	DDO 83
in source:	DDO 214
in source:	DDO 218
in source:	IC 10
Ref:	=1985ApJS...58..533H
by	HUNTER D.A. , GALLAGHER III J.S.
	Astrophys. J., Suppl. Ser., 58, 533-560 (1985)
	Star-forming properties and histories of dwarf irregular galaxies: down but not out.
o	HII regions in IC 1613, M 33, DDO 209, and in table 8 are not [HG85] regions and are not included in Simbad
o	Tables 5, 6, 7: <[HG85] DDO NNN NN>, <[HG85] DDO 49 cen>, <[HG85] IC 10 N> N=74
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HG86]
[HG86]	(Humphreys+Graham, 1986)
Write:	<<[HG86] NN>>
Object:	* (SIMBAD class: Star)
Note:	N=35 red stars in NGC 300 field.
in source:	NGC 300
Ref:	=1986AJ.....91..522H
by	HUMPHREYS R.M. , GRAHAM J.A.
	Astron. J., 91, 522-529 (1986)
	The M supergiants in NGC 300.
o	in ref list CUDWORTH 1984PASP...96..786C instead of 96.789
o	Table 1: <[HG86] NN> (Nos 1-35).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HG90]
[HG90]	(Hunter+Gallagher, 1990)= ([HG90a])
Write:	<<[HG90] NGC NNNN Region NN>> <<[HG90] NGC NNNN Filament N>> <<[HG90] Sex A Filament N>>
N:	17+12
Object:	Region and Filament (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Maps in Figs 1, 2 1st ref.
in source:	NGC 4449
in source:	NGC 4214
in source:	NGC 3738
in source:	NGC 2366
in source:	Sextans A = DDO 75
Ref:	=1990ApJ...362..480H
by	HUNTER D.A. , GALLAGHER III J.S.
	Astrophys. J., 362, 480-490 (1990)
	Properties of ionized interstellar froth in irregular galaxies.
o	Table 2: <[HG90] NGC 4449 Region NN> (Nos 1-14), <[HG90] NGC 4214 Region N> No. 1, <[HG90] NGC 3738 Region N> (Nos 1-2). Table 3: <[HG90] NGC 4449 Filament N> (Nos 1-3), <[HG90] NGC 4214 Filament N> No. 1, <[HG90] NGC 3738 Filament N> No. 1, <[HG90] NGC 2366 Filament N> No. 1, <[HG90] Sex A Filament N> No. 1.
Ref:	=1992ApJ...391L...9H
by	HUNTER D.A. , GALLAGHER III J.S.
	Astrophys. J., 391, 9-12 (1992)
	Supergiant filaments of ionized gas in irregular galaxies.
o	Table 1: <[HG90] NGC 4449 Filament N> (Nos 5-6), <[HG90] Sex A Filament N> (Nos 2-3)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HG90a]
[HG90a]	(Hunter+Gallagher, 1990)
*****	Avoid the usage of [HG90a], prefer [HG90]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HG90b]
[HG90b]	(Hummel+Grave, 1990)
Write:	<<[HG90b] Background NN>> <<[HG90b] Discrete N>>
N:	12+4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio-sources in the field of IC 342. See also [BHJ77].
Ref:	=1990A&A...228..315H
by	HUMMEL E. , GRAVE R.
	Astron. Astrophys., 228, 315-326 (1990)
	The radio continuum emission from IC 342.
o	Table 1: <[HG90b] Background NN> (Nos 1-12). Table 3: <[HG90b] Discrete N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HG99]
[HG99]	(Hric+Galis, 1999)
Write:	<<[HG99] NN>>
N:	17
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Ref:	=1999A&AS..135...29H
by	HRIC L. , GALIS R.
	Astron. Astrophys., Suppl. Ser., 135, 29-40 (1999)
	New periods of variable stars in Cygnus based on a quarter of century of photographic observations.
o	Table 3: <[HG99] NN> (Nos 1-17).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HGAM
HGAM	(Hgamma Catalog)
Write:	<<HGAM NNNN>>
N:	1171
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Hγ catalog for N=1171 stars.
Ref:	=1973PDAO...14..151P
by	PETRIE R.M. , CRAMPTON D., LEIR A., JOUNGER S.
	Publ. Dominion Astrophys. Obs., 14, 151-184 (1973)
	A catalogue of Hγ measures.
o	Table 2: <HGAM NNNN> (Nos 1-1171).
=E=	Catalogue in electronic form as III/29
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGB93]
[HGB93]	(Hertz+Grindlay+Bailyn, 1993)
Write:	<<[HGB93] A>>
N:	8
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations of M 3 = NGC 5272.
in source:	NGC 5272 = M 3
Ref:	=1993ApJ...410L..87H
by	HERTZ P. , GRINDLAY J.E., BAILYN C.D.
	Astrophys. J., 410, 87-90 (1993)
	A supersoft variable low-luminosity X-ray source in the globular cluster M 3.
o	Table 1: <[HGB93] A> (Nos A-F).
Ref:	=2001A&A...368..137V
by	VERBUNT F.
	Astron. Astrophys., 368, 137-159 (2001)
	A census with ROSAT of low-luminosity X-ray sources in globular clusters.
o	Table 2: see also [FLM96], [HCJ97], [HG83b], [HGB93], [JVH94], [JVH96], [RDL94].
o	Table 2: <[V2001] NGC NNNN XNNa> N=49, <[V2001] JHHMMSS.ss+DDMMSS.s> N=2, <[FLM96] M 13 Aa> (Nos F, Ga-Gb, R-T) added, <[HCJ97] NN> (Nos 6-10) added, <[HGB93] A> (No. G) added, <[JVH94] NGC 6626 NNa> (Nos 5-12, 2a-2c) added, <[JVH94] NGC 6656 N> (No. 9) added, <[JVH94] NGC 7099 NN> (No. 13) added, <[JVH96] NGC 6121 NN> (Nos 7-10) added, <[JVH96] NGC 6352 NN> (No. 17) added, <[JVH96] NGC 6366 NN> (Nos 7-8) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HGBS
HGBS	(Herschel Gould Belt survey)
Write:	<<HGBS JHHMMSS.s+DDMMSS>> <<HGBS YSO JHHMMSS.s+DDMMSS>>
N:	749+536+239+532+38+1844+832+833+816+513
Object:	Dense Core + YSO (SIMBAD class: Infrared = Infra-Red Source)
Note:	The Herschel Gould Belt Survey (HGBS) is an extensive imaging survey of the densest portions of the Gould Belt with Herschel SPIRE at 250-500 and PACS at 110-170 microns down to a 5-sigma column sensitivity NH₂∼10²¹cm^–2. The target clouds span a range of physical conditions, from active, cluster-forming complexes to quiescent regions with lower star formation activity. For more information, visit www.herschel.fr/cea/gouldbelt/en/
in source:	NAME Aquila Cloud
in source:	LDN 1495
in source:	NAME CRA MCLD
in source:	NAME Lupus Cloud = NAME Lupus Complex
in source:	NAME Orion B
in source:	LDN 1157
in source:	LDN 1172
in source:	LDN 1228
in source:	LDN 1241
in source:	LDN 1251
in source:	NAME Serpens Cloud
in source:	NAME Perseus Molecular Cloud
in source:	NAME rho Oph Cloud
Ref:	=2015A&A...584A..91K
by	KOENYVES V. , ANDRE Ph., MEN'SHCHIKOV A., PALMEIRIM P., ARZOUMANIAN D., SCHNEIDER N., ROY A., DIDELON P., MAURY A., SHIMAJIRI Y., DI FRANCESCO J., BONTEMPS S., PERETTO N., BENEDETTINI M., BERNARD J.-P., ELIA D., GRIFFIN M.J., HILL T., KIRK J., LADJELATE B., MARSH K., MARTIN P.G., MOTTE F., NGUYEN LUONG Q., PEZZUTO S., ROUSSEL H., RYGL K.L.J., SADAVOY S.I., SCHISANO E., SPINOGLIO L., WARD-THOMPSON D., WHITE G.J.
	Astron. Astrophys., 584A, 91-91 (2015)
	A census of dense cores in the Aquila cloud complex: SPIRE/PACS observations from the Herschel Gould Belt survey.
o	Tables A.1-A.2, col(1): <[KAM2015] NNN> (Nos 1-749) = Tables A.1-A.2, col(2): <HGBS JHHMMSS.s+DDMMSS> N=749.
Ref:	=2016MNRAS.459..342M
by	MARSH K.A. , KIRK J.M., ANDRE P., GRIFFIN M.J., KONYVES V., PALMEIRIM P., MEN'SHCHIKOV A., WARD-THOMPSON D., BENEDETTINI M., BRESNAHAN D.W., DI FRANCESCO J., ELIA D., MOTTE F., PERETTO N., PEZZUTO S., ROY A., SADAVOY S., SCHNEIDER N., SPINOGLIO L., WHITE G.J.
	Mon. Not. R. Astron. Soc., 459, 342-356 (2016)
	A census of dense cores in the Taurus L1495 cloud from the Herschel Gould Belt Survey.
o	Tables B1-B2, col(2): <HGBS JHHMMSS.s+DDMMSS> N=536.
Ref:	=2018A&A...615A.125B
by	BRESNAHAN D. , WARD-THOMPSON D., KIRK J.M., PATTLE K., EYRES S., WHITE G.J., KONYVES V., MEN'SHCHIKOV A., ANDRE P., SCHNEIDER N., DI FRANCESCO J., ARZOUMANIAN D., BENEDETTINI M., LADJELATE B., PALMEIRIM P., BRACCO A., MOLINARI S., PEZZUTO S., SPINOGLIO L.
	Astron. Astrophys., 615A, 125-127 (2018)
	The dense cores and filamentary structure of the molecular cloud in Corona Australis: Herschel SPIRE and PACS observations from the Herschel Gould Belt Survey.
o	Fig.5 Regions A-F not in SIMBAD.
o	Tables A.1-A.2, col(2): <HGBS JHHMMSS.s+DDMMSS> N=239.
Ref:	=2018A&A...619A..52B
by	BENEDETTINI M. , PEZZUTO S., SCHISANO E., ANDRE P., KONYVES V., MEN'SHCHIKOV A., LADJELATE B., DI FRANCESCO J., ELIA D., ARZOUMANIAN D., LOUVET F., PALMEIRIM P., RYGL K.L.J., SCHNEIDER N., SPINOGLIO L., WARD-THOMPSON D.
	Astron. Astrophys., 619A, 52-52 (2018)
	A catalogue of dense cores and young stellar objects in the Lupus complex based on Herschel Gould Belt Survey observations.
o	Tables A.1-A.2: <HGBS JHHMMSS.s+DDMMSS> N=532. Table B.1: <HGBS YSO JHHMMSS.s+DDMMSS> N=38.
Ref:	=2020A&A...635A..34K
by	KONYVES V. , ANDRE P., ARZOUMANIAN D., SCHNEIDER N., MEN'SHCHIKOV A., BONTEMPS S., LADJELATE B., DIDELON P., PEZZUTO S., BENEDETTINI M., BRACCO A., DI FRANCESCO J., GOODWIN S., RYGL K.L.J., SHIMAJIRI Y., SPINOGLIO L., WARD-THOMPSON D., WHITE G.J.
	Astron. Astrophys., 635A, 34-34 (2020)
	Properties of the dense core population in Orion B as seen by the Herschel Gould Belt survey.
o	Tables A.1-A.2: <HGBS JHHMMSS.s+DDMMSS> N=1844. Table A.1: <[KAA2020] JHHMMSS.s+DDMMSS> N=26.
Ref:	=2020ApJ...904..172D
by	DI FRANCESCO J. , KEOWN J., FALLSCHEER C., ANDRE P., LADJELATE B., KONYVES V., MEN'SHCHIKOV A., STEPHENS-WHALE S., NGUYEN-LUONG Q., MARTIN P., SADAVOY S., PEZZUTO S., FIORELLINO E., BENEDETTINI M., SCHNEIDER N., BONTEMPS S., ARZOUMANIAN D., PALMEIRIM P., KIRK J.M., WARD-THOMPSON D.
	Astrophys. J., 904, 172-172 (2020)
	Herschel Gould Belt Survey observations of dense cores in the Cepheus Flare clouds.
o	Tables C1-C2: <HGBS JHHMMSS.s+DDMMSS> N=832.
Ref:	=2021MNRAS.500.4257F
by	FIORELLINO E. , ELIA D., ANDRE P., MEN'SHCHIKOV A., PEZZUTO S., SCHISANO E., KONYVES V., ARZOUMANIAN D., BENEDETTINI M., WARD-THOMPSON D., BRACCO A., DI FRANCESCO J., BONTEMPS S., KIRK J., MOTTE F., MOLINARI S.
	Mon. Not. R. Astron. Soc., 500, 4257-4276 (2021)
	The census of dense cores in the Serpens region from the Herschel Gould Belt Survey.
o	Tables A1-A2: <HGBS JHHMMSS.s+DDMMSS> N=833.
Ref:	=2021A&A...645A..55P
by	PEZZUTO S. , BENEDETTINI M., DI FRANCESCO J., PALMEIRIM P., SADAVOY S., SCHISANO E., LI CAUSI G., ANDRE P., ARZOUMANIAN D., BERNARD J.-P., BONTEMPS S., ELIA D., FIORELLINO E., KIRK J.M., KONYVES V., LADJELATE B., MEN'SHCHIKOV A., MOTTE F., PICCOTTI L., SCHNEIDER N., SPINOGLIO L., WARD-THOMPSON D., WILSON C.D.
	Astron. Astrophys., 645A, 55-55 (2021)
	Physical properties of the ambient medium and of dense cores in the Perseus star-forming region derived from Herschel Gould Belt Survey observations.
o	Tables A.1-A.3: <HGBS JHHMMSS.s+DDMMSS> N=816. Tables E.1-E.3: <[PBD2021] NNN> (Nos 1-170).
o	Table 5, Fig.9 HPZ regions not identified.
Ref:	=2020A&A...638A..74L
by	LADJELATE B. , ANDRE P., KONYVES V., WARD-THOMPSON D., MEN'SHCHIKOV A., BRACCO A., PALMEIRIM P., ROY A., SHIMAJIRI Y., KIRK J.M., ARZOUMANIAN D., BENEDETTINI M., DI FRANCESCO J., FIORELLINO E., SCHNEIDER N., PEZZUTO S., MOTTE F., (The Herschel Gould Belt Survey Team Collaboration)
	Astron. Astrophys., 638A, 74-74 (2020)
	The Herschel view of the dense core population in the Ophiuchus molecular cloud.
o	Tables A.1-A.2: <HGBS JHHMMSS.s+DDMMSS> N=513.
=E=	Catalogue in electronic form as <J/A+A/584/A91/>
=E=	Catalogue in electronic form as <J/MNRAS/459/342/>
=E=	Catalogue in electronic form as <J/A+A/615/A125/>
=E=	Catalogue in electronic form as <J/A+A/619/A52/>
=E=	Catalogue in electronic form as <J/A+A/635/A34/>
=E=	Catalogue in electronic form as <J/A+A/645/A55/>
=E=	Catalogue in electronic form as <J/A+A/638/A74/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HGC2012]
[HGC2012]	(Harbeck+Gallagher III+Crnojevic, 2013) (Not yet in Simbad)
Write:	<<[HGC2012] NNN>>
N:	31
Object:	Poss. Cluster of * (SIMBAD class: Cluster*_Candidate = Cluster of Stars Candidate)
Note:	N=29+2 cluster candidates in NGC 5253. Use of HST ACS archival data.
in source:	NGC 5253
Ref:	=2012MNRAS.422..629H
by	HARBECK D. , GALLAGHER III J., CRNOJEVIC D.
	Mon. Not. R. Astron. Soc., 422, 629-636 (2012)
	Intermediate old star clusters in a young starburst: the case of NGC 5253.
o	Fig. 1, Table 2: <[HGC2012] NNN> (Nos 1-29, 102-103).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HGCG
HGCG	(Huchra+Geller, Cluster of G)
*****	Avoid the usage of HGCG, prefer [HG82]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [HGD2002]
[HGD2002]	(Hatziminaoglou+Groenewegen+Da Costa+, 2002)= (EIS)
Write:	<<[HGD2002] EIS JHHMMSS.ss+DDMMSS.s>>
N:	234+97+53+20
Object:	QSO + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	EIS of the CDFS: N=234 QSO candidates, N=97 white dwarfs candidates, N=53 low-mass stars candidates, N=20 Very Red Objects.
in source:	NAME CDFS
Ref:	=2002A&A...384...81H
by	HATZIMINAOGLOU E. , GROENEWEGEN M.A.T., DA COSTA L., ARNOUTS S., BENOIST C., MADEJSKY R., MIGNANI R.P., OLSEN L.F., RITE C., SCHIRMER M., SLIJKHUIS R., VANDAME B.
	Astron. Astrophys., 384, 81-98 (2002)
	ESO Imaging Survey. Exploring the optical/infrared imaging data of CDF-S: Point sources.
o	Tables 1 to 4: <[HGD2002] EIS JHHMMSS.ss+DDMMSS.s> N=234+97+53+20.
=E=	Catalogue in electronic form as J/A+A/384/81
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGD90]
[HGD90]	(Huchra+Geller+De Lapparent+, 1990) (Not yet in Simbad)
Write:	<<[HGD90] HHMM+DDMM>> <<[HGD90] HHMM+DDMMA>> <<[HGD90] HHMM+DDMMW>>
N:	667
Object:	G (SIMBAD class: Galaxy)
Note:	CfA redshift survey for the NGP zone. N=667 among the 1093 of the complete catalogue. See [HVG99b] for the SGP zone.
Ref:	=1990ApJS...72..433H
by	HUCHRA J.P. , GELLER M.J., DE LAPPARENT V., CORWIN H.G.Jr
	Astrophys. J., Suppl. Ser., 72, 433-470 (1990)
	The CfA redshift survey : data for the NGP + 30 zone.
o	Catalogue: <[HGD90] HHMM+DDMM>, <[HGD90] HHMM+DDMMA>, <[HGD90] HHMM+DDMMW>, N=667.
=E=	Catalogue in electronic form as VII/193
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGE2003]
[HGE2003]	(Heinke+Grindlay+Edmonds+, 2003)
Write:	<<[HGE2003] CXNN>>
N:	19
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of the globlular cluster M 80.
in source:	NGC 6093 = M 80
Ref:	=2003ApJ...598..516H
by	HEINKE C.O. , GRINDLAY J.E., EDMONDS P.D., LLOYD D.A., MURRAY S.S., COHN H.N., LUGGER P.M.
	Astrophys. J., 598, 516-526 (2003)
	A Chandra X-ray study of the globular cluster M80.
o	Table 1: <[HGE2003] CXNN> (Nos CX1 to CX19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGF2018]
[HGF2018]	(Hlavacek-Larrondo+Gendron-Marsolais+Fecteau-Beaucage+, 2018)
Write:	<<[HGF2018] SN>>
N:	9
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Karl G. Jansk VLA 1-2 GHz observations of N=9 radio-sources in the ACO 2146 galaxy cluster.
in source:	ACO 2146
Ref:	=2018MNRAS.475.2743H
by	HLAVACEK-LARRONDO J. , GENDRON-MARSOLAIS M.-L., FECTEAU-BEAUCAGE D., VAN WEEREN R.J., RUSSELL H.R., EDGE A., OLAMAIE M., RUMSEY C., KING L., FABIAN A.C., McNAMARA B., HOGAN M., MEZCUA M., TAYLOR G.
	Mon. Not. R. Astron. Soc., 475, 2743-2753 (2018)
	Mystery solved: discovery of extended radio emission in the merging galaxy cluster Abell 2146.
o	Table 2, Fig. 2: <[HGF2018] SN> (Nos S1-S9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGG2004]
[HGG2004]	(Harbeck+Gallagher III+Grebel, 2004)
Write:	<<[HGG2004] aaaN-NNNNN>> <<[HGG2004] aaaaa-RNNNN>>
N:	1+2+5+3
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Note:	Results of a photometric survey with the WIYN telescope for carbon stars in companions of M 31 (And III, And VI, And VII). Observations with two chips (I and II in the format) in Cetus dwarf galaxy.
in source:	And III
in source:	And VI
in source:	And VII
in source:	NAME Cetus Dwarf Galaxy
Ref:	=2004AJ....127.2711H
by	HARBECK D. , GALLAGHER III J.S., GREBEL E.K.
	Astron. J., 127, 2711-2722 (2004)
	WIYN survey for carbon stars in the M31 and Cetus dwarf spheroidal galaxies: evolutionary implications.
o	Table 1: <[HGG2004] andN-NNNNN> N=1+2+5, <HGG2004] cetus-RNNNN> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGG90]
[HGG90]	(Hodge+Gurwell+Goldader+, 1990)
*****	Avoid the usage of [HGG90], prefer HGGK
Origin	of the Acronym: S = Created by Simbad, the CDS Database
History	of this Acronym: replaced by HGGK
Details on Acronym: [HGG98]
[HGG98]	(Hasinger+Giacconi+Gunn+, 1998)
Write:	<<[HGG98] A>> <<[HGG98] NN>>
N:	4+24
Object:	(X) + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	ROSAT Deep Survey and Keck LHRI observations. Table 1: (Nos A-D), N=4 X-ray sources near RX J1053.7+5735. A+B = Cluster of G, C = Group of G. Table 2: (Nos 1-24), N=24 galaxies in the field of RX J1053.7+5735. Map in Fig.1. See also RDS and [ZMH99].
Ref:	=1998A&A...340L..27H
by	HASINGER G. , GIACCONI R., GUNN J.E., LEHMANN I., SCHMIDT M., SCHNEIDER D.P., TRUEMPER J., WAMBSGANSS J., WOODS D., ZAMORANI G.
	Astron. Astrophys., 340, 27-30 (1998)
	The ROSAT Deep Survey. IV. A distant lensing cluster of galaxies with a bright arc.
o	lensing cluster of galaxies = ClG J1053+5735, Bright arc = [HGG98] 2.
o	Table 1: <[HGG98] A> (Nos A-D). Table 2: <[HGG98] NN> (Nos 1-24).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HGGK
HGGK	(Hodge+Gurwell+Goldader+Kennicutt)= ([HGG90])
Write:	<<HGGK NNNN>>
N:	1264
Object:	HII (SIMBAD class: HIIReg = HII Region)
in source:	M 101 = NGC 5457
Ref:	=1990ApJS...73..661H
by	HODGE P.W. , GURWELL M., GOLDADER J.D., KENNICUTT R.C.
	Astrophys. J., Suppl. Ser., 73, 661-670 (1990)
	The HII regions of M 101. I. An atlas of 1264 emission regions.
o	<HGGK NNNN> (Nos 1-1264).
=E=	Catalogue in electronic form as J/ApJS/73/661
Origin	of the Acronym: L (1995AJ....110.2088M)
Details on Acronym: [HGH2004]
[HGH2004]	(Harris+Geisler+Harris+, 2004)
Write:	<<[HGH2004] DDD.ddddd+DD.ddddd>>
N:	about 106000
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Big Throughput Camera (BTC) at the Cerro Tololo Inter-American observatory 4m telescope observations of the field around Cen A = NGC 5128. Study of the globular cluster system (GCS). See [HHG2004]
in source:	Cen A = NGC 5128
Ref:	=2004AJ....128..712H
by	HARRIS G.L.H. , GEISLER D., HARRIS W.E., SCHMIDT B.P., HESSER J.E., REID M., MILNE M., HULME S.C., KIDD T.T.
	Astron. J., 128, 712-722 (2004)
	Wide-field Washington photometry of the NGC 5128 globular cluster system. I. The database.
o	Table 3: <[HGH2004] DDD.ddddd+DD.ddddd> N about 106000.
=E=	Catalogue in electronic form as J/AJ/128/712
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGH2007]
[HGH2007]	(Helfand+Gotthelf+Halpern+, 2007)
Write:	<<[HGH2007] NN>>
N:	75
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra X-ray observations of the field of the gamma source HESS J1813-178.
Ref:	=2007ApJ...665.1297H
by	HELFAND D.J. , GOTTHELF E.V., HALPERN J.P., CAMILO F., SEMLER D.R., BECKER R.H., WHITE R.L.
	Astrophys. J., 665, 1297-1303 (2007)
	Discovery of the putative pulsar and wind nebula associated with the TeV γ-ray source HESS J1813-178.
o	Table 1: <[HGH2007] NN> (Nos 1-75).
=E=	Catalogue in electronic form as J/ApJ/665/1297
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGH2008]
[HGH2008]	(Hennekemper+Gouliermis+Henning+, 2008)
Write:	<<[HGH2008] Cluster Na>>
N:	6
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST ACS observations. N=6 clusters of PMS* near NGC 346.
in source:	Magellanic CLouds:SMC = SMC
Ref:	=2008ApJ...672..914H
by	HENNEKEMPER E. , GOULIERMIS D.A., HENNING T., BRANDNER W., DOLPHIN A.E.
	Astrophys. J., 672, 914-929 (2008)
	NGC 346 in the Small Magellanic Cloud. III. Recent star formation and stellar clustering properties in the bright H II region N66.
o	Fig. 10: <[HGH2008] Cluster Na> (Nos 1, 2a-2b, 3-5).
=E=	Catalogue in electronic form as J/ApJ/672/914
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGH2012]
[HGH2012]	(Harris+Gomez+Harriz+, 2012)
Write:	<<[HGH2012] DDD.ddddddd+DD.ddddddd>>
N:	833
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	Magellan Baade telescope IMACS observations of N=833 globular cluster candidates around NGC 5128.
in source:	Cen A = NGC 5128
Ref:	=2012AJ....143...84H
by	HARRIS G.L.H. , GOMEZ M., HARRIS W.E., JOHNSTON K., KAZEMZADEH F., KERZENDORF W., GEISLER D., WOODLEY K.A.
	Astron. J., 143, 84 (2012)
	Eight hundred new candidates for globular clusters in NGC 5128 (Centaurus A).
o	Table 1: <[HGH2012] DDD.ddddddd+DD.ddddddd> N=833.
=E=	Catalogue in electronic form as <J/AJ/143/84/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGH92]
[HGH92]	(Harris+Geisler+Harris+, 1992)= (G) = (H92) = (HGHH) = (HGHH92)
Write:	<<[HGH92] GNNN>>
N:	33
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	Liste 'GNNN' of Globular clusters, described in Sharples, 1988IAUS..126..545S
in source:	Cen A = NGC 5128
Ref:	=1992AJ....104..613H
by	HARRIS G.L.H. , GEISLER D., HARRIS H.C., HESSER J.E.
	Astron. J., 104, 613-626 (1992)
	Metal abundances from Washington photometry of globular clusters in NGC 5128.
o	The list of globular clusters '[HGH92]' is described in 1988IAUS..126..545S
o	Table 1: <[HGH92] GNNN> N=32 among (Nos 19-378). Table 1: <[VHH81] NN> (Nos 40-48, 51) added
Ref:	=1995Msngr..82...22M
by	MINNITI D. , ALONSO M.V., GOUDFROOIJ P., MEYLAN G., JABLONKA P.
	The Messenger, 82, 22-24 (1995)
	New globular clusters identified in the inner regions of NGC 5128 using ESO and HST data.
o	Table 1: <[MAG95] NN> (Nos 1-32). Table 1: <[HGH92] GNNN> (No. G242) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGH95]
[HGH95]	(Henry+Gioia+Huchra+, 1995)
Write:	<<[HGH95] JHHMMSS+DDMMSS>> <<[HGH95] JHHMMSS.s+DDMMSS>>
N:	31
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
in source:	RX J1724.0+7000
in source:	RX J1733.0+7045
in source:	RX J1736.0+6804
in source:	RX J1744.0+6633
in source:	RX J1751.0+6532
in source:	RX J1755.0+6236
in source:	RX J1756.0+6512
in source:	RX J1833.0+6520
Ref:	=1995ApJ...449..422H
by	HENRY J.P. , GIOIA I.M., HUCHRA J.P., BURG R., McLEAN B., BOHRINGER H., BOWER R.G., BRIEL U.G., VOGES W., MacGILLIVRAY H., CRUDDACE R.G.
	Astrophys. J., 449, 422-430 (1995)
	Groups of galaxies in the ROSAT north ecliptic pole survey.
o	Table 1: <[HGH95] JHHMMSS+DDMMSS>, <[HGH95] JHHMMSS.s+DDMMSS> N=31
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HGHH
HGHH	(Harris+Geisler+Harris+Hesser)
*****	Avoid the usage of HGHH, prefer [HGH92]
Origin	of the Acronym: L (2004ApJS..150..367P)
Details on Acronym: HGHH
HGHH	(Harris+Geisler+Harris+Hesser)
*****	Avoid the usage of HGHH, prefer [VHH81]
Origin	of the Acronym: L (2004ApJS..150..367P)
Details on Acronym: HGHH92
HGHH92	(Harris+Geisler+Harris+Hesser, 1992)
*****	Avoid the usage of HGHH92, prefer [HGH92]
Origin	of the Acronym: L (2007A&A...469..147R)
Details on Acronym: [HGJ99]
[HGJ99]	(Huang+Gu+Ji+, 1999) (Not yet in Simbad)
Write:	<<[HGJ99] N>>
N:	4
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	N=4 sources in the field of IRAS F08208+2816. (Nos 1-3) are components of IRAS system, (No. 4) is a foreground star.
Ref:	=1999ApJ...513..215H
by	HUANG J.H. , GU Q.S., JI L., LI W.D., WEI J.Y., ZHENG W.
	Astrophys. J., 513, 215-223 (1999)
	New Wolf-Rayet galaxies with detection of WC stars.
o	Fig.6: <[HGJ99] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGL2001]
[HGL2001]	(Halpern+Gotthelf+Leighly+, 2001)
Write:	<<[HGL2001] J2229.0+6114 Star A>> <<[HGL2001] VLA J2229.0+6114>>
N:	2
Object:	* + (Rad) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Near RX J2229.0+6114, N=1 Star 'A', and N=1 radio shell including the RX, 'VLA J2229.0+6114'.
Ref:	=2001ApJ...547..323H
by	HALPERN J.P. , GOTTHELF E.V., LEIGHLY K.M., HELFAND D.J.
	Astrophys. J., 547, 323-333 (2001)
	A possible X-ray and radio counterpart of the high-energy γ-ray source 3EG J2227+6122.
o	Fig.3: <[HGL2001] J2229.0+6114 Star A> (No. A). Figs 4, 5: <[HGL2001] VLA J2229.0+6114> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGM2009]
[HGM2009]	(Huang+Gies+McSwain, 2009)= ([HGM2009a])
Write:	<<[HGM2009] JHHMMSS.ss+DDMMSS.s>>
N:	12
Object:	High Velocity * (SIMBAD class: HighVel* = High Velocity Star)
Stat:	is completely incorporated in Simbad
Note:	KPNO 2.1m telescope spectroscopic observations of the projected trajectory of HD 69686.
Ref:	=2009ApJ...703...81H
by	HUANG W. , GIES D.R., McSWAIN M.V.
	Astrophys. J., 703, 81-88 (2009)
	HD 69686: a mysterious high velocity b star.
o	Table 6: <[HGM2009] JHHMMSS.ss+DDMMSS.s> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGM2009a]
[HGM2009a]	(Huang+Gies+McSwain, 2009)
*****	Avoid the usage of [HGM2009a], prefer [HGM2009]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGM2009b]
[HGM2009b]	(Hole+Geller+Mathieu+, 2009)= (WOCS)
Write:	<<[HGM2009b] WOCS NNNFFF>>
N:	2706
Object:	* (SIMBAD class: Star)
Note:	Radial velocity measurements in NGC 6819 from the WIYN Open Cluster Study (WOCS). The identification number is the three digit star number followed by the three digit annulus number.
in source:	NGC 6819
Ref:	=2009AJ....138..159H
by	HOLE K.T. , GELLER A.M., MATHIEU R.D., PLATAIS I., MEIBOM S., LATHAM D.W.
	Astron. J., 138, 159-168 (2009)
	WIYN open cluster study. XXIV. Stellar radial-velocity measurements in NGC 6819.
o	Tables 1-2: <[HGM2009b] WOCS NNNFFF> N=1418 among (Nos 1001-115030).
Ref:	=2014AJ....148...38M
by	MILLIMAN K.E. , MATHIEU R.D., GELLER A.M., GOSNELL N.M., MEIBOM S., PLATAIS I.
	Astron. J., 148, 38 (2014)
	WIYN open cluster study. LX. Spectroscopic binary orbits in NGC 6819.
o	Tables 1-2, 5-6: <[HGM2009b] WOCS NNNFFF> N=2641 among (Nos 1001-260043).
=E=	Catalogue in electronic form as <J/AJ/138/159/>
=E=	Catalogue in electronic form as J/AJ/148/38
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGM93]
[HGM93]	(Heydari-Malayeri+Grebel+Melnick+, 1993)= (HM) = (H-M)
Write:	<<[HGM93] NNAa>>
N:	31+9+2
Object:	* (SIMBAD class: Star)
Note:	Format 'NN', (Nos 3-33), some stars been resolved in several formats 'NNA', and star 5A been itself resolved in 2 '5Aa' and '5Ab'.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1993A&A...278...11H
by	HEYDARI-MALAYERI M. , GREBEL E.K., MELNICK J., JORDA L.
	Astron. Astrophys., 278, 11-22 (1993)
	HDE 269828 : a reddened massive star cluster.
o	<[HGM93] NN> N=31 (Nos 3-33)
Ref:	=1995ApJ...439L..47W
by	WALBORN N.R. , MacKENTY J.W., SAHA A., WHITE R.L., PARKER J.W.
	Astrophys. J., 439, 47-50 (1995)
	Resolution of massive compact clusters in the 30 Doradus periphery with the Hubble space telescope.
o	Table 1: <[TLD88] NNA> (Nos 1A-1C, 2A-2C), <[HGM93] NNA> (Nos 5A-5C, 9A-9B, 11A-11B), <[ST92] 2-NNA> (Nos 62A-62B, 67A-67B, 69A-69B).
Ref:	=1999AJ....118.1684W
by	WALBORN N.R. , DRISSEN L., PARKER J.W., SAHA A., MacKENTY J.W., WHITE R.L.
	Astron. J., 118, 1684-1699 (1999)
	HST/FOS spatially resolved spectral classification of compact OB groups in the Large Magellanic Cloud.
o	LH 10-3209 is [L72] LH 10-3209 = PGMW 3209 in SIMBAD.
o	Table 1: <[WDP99] Brey 73 NN> N=23 among (Nos 1-28). Table 2: <[WDP99] NGC 2044W NN> N=37 among (Nos 1-45). Table 3: <[WDP99] LH 10-3209 NN> (Nos 14-19) = <[WDP99] LH 10-3209 A> (Nos A-F). Table 4: <[WDP99] HD 32228 NN> N=71 among (Nos 1-98). Fig.5, Table 2: <[HGM93] NNAa> (Nos 5Aa, 5Ab, 5D, 5E) added. Fig.12, Table 4: <[HT83] HD 32228 aN> (Nos b1-b2, g1-g3, h1-h2) added.
=E=	Catalogue in electronic form as <J/AJ/118/1684/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGM97]
[HGM97]	(Henry+Gioia+Mullis+, 1997)
Write:	<<[HGM97] NN>>
N:	12
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	ROSAT HRI observations of a cluster of galaxies, from ROSAT NEP survey. N=12 galaxies cluster members. Finding chart Fig.1
in source:	RX J1716.0+6708
Ref:	=1997AJ....114.1293H
by	HENRY J.P. , GIOIA I.M., MULLIS C.R., CLOWE D.I., LUPPINO G.A., BOEHRINGER H., BRIEL U.G., VOGES W., HUCHRA J.P.
	Astron. J., 114, 1293-1296 (1997)
	Discovery of a redshift 0.8 cluster of galaxies in the ROSAT North Ecliptic Pole Survey.
o	Table 1: <[HGM97] NN> (Nos 1-12)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGO2008]
[HGO2008]	(Hennawi+Gladders+Oguri+, 2008)
Write:	<<[HGO2008] SDSS JHHMM+DDMM>>
N:	9+8+4
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	WIYN and UH88 observations of distant clusters.
Ref:	=2008AJ....135..664H
by	HENNAWI J.F. , GLADDERS M.D., OGURI M., DALAL N., KOESTER B., NATARAJAN P., STRAUSS M.A., INADA N., KAYO I., LIN H., LAMPEITL H., ANNIS J., BAHCALL N.A., SCHNEIDER D.P.
	Astron. J., 135, 664-681 (2008)
	A new survey for giant arcs.
o	Tables 1-3: <[HGO2008] SDSS JHHMM+DDMM> N=9+8+4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGP2002]
[HGP2002]	(Homeier+Gallagher+Pasquali, 2002)
Write:	<<[HGP2002] ANN>> <<[HGP2002] fNN>>
N:	12+8+12+18
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	Archival HST WFPC2 data. Study of the star cluster system in NGC 7673. In the format, the letter 'A' stands for A, B, C, Cl* in [DA82] Clump A, B, C. Format 'fNN' stands for field Cl* not associated with a peculiar clump.
in source:	NGC 7673
Ref:	=2002A&A...391..857H
by	HOMEIER N. , GALLAGHER III J.S., PASQUALI A.
	Astron. Astrophys., 391, 857-873 (2002)
	The star cluster system of the NGC 7673 starburst.
o	Fig.9, Table 2: <[HGP2002] ANN> (Nos A1-A12, B1-B8, C1-C12), <[HGP2002] aNN> (Nos f1-f18).
=E=	Catalogue in electronic form as J/A+A/391/857
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGP92]
[HGP92]	(Harris+Guetter+Pier+, 1992)
Write:	<<[HGP92] NGC NNNN HHMMSS.ss+DDMMSS.s>> <<[HGP92] PAL NN HHMMSS.ss+DDMMSS.s>>
N:	130
Object:	(Rad) in GCl (SIMBAD class: Radio = Radio Source)
Note:	Table 2: Radio-sources in 36 NGC globular clusters: format 'NGC NNNN HHMMSS.ss+DDMMSS.s, and 3 Palomar clusters Pal 5, Pal 11, Pal 12: format 'PAL NN HHMMSS.ss+DDMMSS.s,
Ref:	=1992AJ....104...53H
by	HARRIS H.C. , GUETTER H.H., PIER J.R., ABLES H.D., MONET D.G., FOLTZ C.B., CHAFFEE F.H., BOYLE B.J., IRWIN M.J.
	Astron. J., 104, 53-62 (1992)
	A search for QSOs behind globular clusters.
o	Table 2: <[HGP92] NGC NNNN HHMMSS.ss+DDMMSS.s> and <[HGP92] PAL NN HHMMSS.ss+DDMMSS.s> N=130
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGR2010]
[HGR2010]	(Held+Gullieuszik+Rizzi+, 2010)
Write:	<<[HGR2010] NNNNNN>>
N:	7471
Object:	* (SIMBAD class: Star)
Note:	UKIRT WFCAM observations of the dwarf spheroidal galaxy Leo I.
in source:	UGC 5470 = Leo I
Ref:	=2010MNRAS.404.1475H
by	HELD E.V. , GULLIEUSZIK M., RIZZI L., GIRARDI L., MARIGO P., SAVIANE I.
	Mon. Not. R. Astron. Soc., 404, 1475-1489 (2010)
	A near-infrared study of AGB and red giant stars in the Leo I dSph galaxy.
o	Table 2: <[HGR2010] NNNNNN> N=7471 among (Nos 41-200324).
=E=	Catalogue in electronic form as J/MNRAS/404/1475
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGS97]
[HGS97]	(Hammer+Gioia+Shaya+, 1997) (Not yet in Simbad)
Write:	<<[HGS97] SN>> <<[HGS97] A>>
N:	3+5
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST WFPC2 images of the cluster of galaxies 1E 2137.3-2353. Fig.5: sources (Nos S1-S3): Sources of arc images in [FLH92]. Fig.5: 5 knots (Nos A-E).
in source:	1E 2137.0-2353
Ref:	=1997ApJ...491..477H
by	HAMMER F. , GIOIA I.M., SHAYA E.J., TEYSSANDIER P., LE FEVRE O., LUPPINO G.A.
	Astrophys. J., 491, 477-482 (1997)
	Detailed lensing properties of the MS 2137-2353 core and reconstruction of sources from Hubble Space Telescope imagery.
o	Fig.2: <[FLH92] AR> N=1 added, <[FLH92] ARN> N=1 added, <[FLH92] A01 SKN> (Nos SK1-SK2) added, <[FLH92] A02 SKN> (Nos SK1-SK2) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HGT
HGT	(Halpern+Grindlay+Tytler)
Write:	<<HGT NNN>>
N:	61+76
Object:	* (SIMBAD class: Star)
Note:	(Nos 1-61) in the first ref., (Nos 101-176) in the second ref. Identif. charts
Ref:	=1985ApJ...296..190H
by	HALPERN J.P. , GRINDLAY J.E., TYTLER D.
	Astrophys. J., 296, 190-196 (1985)
	Observations of the Geminga optical candidate.
o	<HGT NN> (Nos 1-61)
Ref:	=1988ApJ...330..201H
by	HALPERN J.P. , TYTLER D.
	Astrophys. J., 330, 201-217 (1988)
	The Geminga X-ray counterpart and a blue optical identification.
o	<HGT NNN> (Nos 101-176)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HGT2015]
[HGT2015]	(Ho+Geha+Tollerud+, 2015)
Write:	<<[HGT2015] M32 NN>> <<[HGT2015] NGC205 NNN>> <<[HGT2015] NGC185 NNN>> <<[HGT2015] NGC147 NNN>> <<[HGT2015] AndVII NNN>> <<[HGT2015] AndII NNN>>
N:	1243
Object:	RGB* (SIMBAD class: RGB* = Red Giant Branch star)
Stat:	is completely incorporated in Simbad
Note:	Keck II DEIMOS observations of N=64+224+321+230+104+300 red giant branch member stars for the six most luminous M31 dwarf galaxy satellites: M32, NGC 205, NGC 185, NGC 147, Andromeda VII and Andromeda II.
Ref:	=2015ApJ...798...77H
by	HO N. , GEHA M., TOLLERUD E.J., ZINN R., GUHATHAKURTA P., VARGAS L.C.
	Astrophys. J., 798, 77 (2015)
	Metallicity evolution of the six most luminous M31 dwarf satellites.
o	Table 2: <[HGT2015] M32 NN> (Nos 1-64), <[HGT2015] NGC205 NNN> (Nos 1-224), <[HGT2015] NGC185 NNN> (Nos 1-321), <[HGT2015] NGC147 NNN> (Nos 1-230), <[HGT2015] AndVII NNN> (Nos 1-104), <[HGT2015] AndII NNN> (Nos 1-300).
=E=	Catalogue in electronic form as J/ApJ/798/77
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGT80]
[HGT80]	(Hoessel+Gunn+Thuan, 1980)
Write:	<<[HGT80] ACO NNNN BCG>>
N:	116
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	N=116 Brightest Cluster Galaxies (BCG) in 116 ACO
Ref:	=1980ApJ...241..486H
by	HOESSEL J.G. , GUNN J.E., THUAN T.X.
	Astrophys. J., 241, 486-492 (1980)
	The photometry properties of brightest cluster galaxies. I. Absolute magnitudes in 116 nearby Abell clusters.
o	Table 1: <[HGT80] ACO NNNN BCG> N=116
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGV2016]
[HGV2016]	(Hardcastle+Gurkan+van Weeren+, 2016)
Write:	<<[HGV2016] JHHMMSS.ss+DDMMSS.s>>
N:	15292
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	LOFAR 126-173MHz observations of N=15292 sources in the North Galactic Pole field.
in source:	NAME NGP
Ref:	=2016MNRAS.462.1910H
by	HARDCASTLE M.J. , GURKAN G., VAN WEEREN R.J., WILLIAMS W.L., BEST P.N., DE GASPERIN F., RAFFERTY D.A., READ S.C., SABATER J., SHIMWELL T.W., SMITH D.J.B., TASSE C., BOURNE N., BRIENZA M., BRUGGEN M., BRUNETTI G., CHYZY K.T., CONWAY J., DUNNE L., EALES S.A., MADDOX S.J., JARVIS M.J., MAHONY E.K., MORGANTI R., PRANDONI I., ROTTGERING H.J.A., VALIANTE E., WHITE G.J.
	Mon. Not. R. Astron. Soc., 462, 1910-1936 (2016)
	LOFAR/H-ATLAS: a deep low-frequency survey of the Herschel-ATLAS North Galactic Pole field.
o	Table A1: <[HGV2016] JHHMMSS.ss+DDMMSS.s> N=15292.
=E=	Catalogue in electronic form as <J/MNRAS/462/1910/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGW89]
[HGW89]	(Hayward+Grasdalen+Woodward+, 1989)
Write:	<<[HGW89] W 3 Star A>>
N:	5
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	W 3
Ref:	=1989ApJ...345..894H
by	HAYWARD T.L. , GRASDALEN G.L., WOODWARD C.E., HACKWELL J.A., GEHRZ R.D., PIPHER J.L.
	Astrophys. J., 345, 894-905 (1989)
	Infrared imaging of the compact HII region W3A.
o	Table 2: <[WBN72] W 3 IRS NNa> (Nos 2b-2c, 11). Table 2: <[HGW89] W 3 Star A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HGZ2018]
[HGZ2018]	(Hunter+Gallardo+Zhang+, 2018)
Write:	<<[HGZ2018] N>>
N:	6
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	Use of HST ACS data to search for star clusters in DDO 187.
in source:	DDO 187
Ref:	=2018ApJ...855....7H
by	HUNTER D.A. , GALLARDO S., ZHANG H.-X., ADAMO A., COOK D.O., OH S.-H., ELMEGREEN B.G., KIM H., KAHRE L., UBEDA L., BRIGHT S.N., RYON J.E., FUMAGALLI M., SACCHI E., KENNICUTT R.C., TOSI M., DALE D.A., CIGNONI M., MESSA M., GREBEL E.K., GOULIERMIS D.A., SABBI E., GRASHA K., GALLAGHER J.S., CALZETTI D., LEE J.C.
	Astrophys. J., 855, 7-7 (2018)
	A study of two dwarf irregular galaxies with asymmetrical star formation distributions.
o	Table 2: <[HGZ2018] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HH
HH	(Herbig-Haro obj.)
*****	Avoid the usage of HH, prefer [ASS79]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HH
HH	(Harris+Geisler)
*****	Avoid the usage of HH, prefer [BBP2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HH
HH	(Herbig Haro obj.)
Write:	<<HH NNNNA>> <<HH NNNNA'>> <<HH NNNNa>> <<HH NNNNANN>> <<HH NNNNAA>> <<HH NNNNAW>> <<HH NNNNAaNN>> <<HH NNNNaN>> <<HH NNNNWA>> <<HH NNNNWW>> <<HH NNNNWWW>> <<HH NNNNWWN>> <<HH NNNNWWNA>>
N:	1120
Object:	HH (SIMBAD class: HerbigHaroObj = Herbig-Haro Object)
Note:	Numerous subdivisions (may be A, AN, AW where W stands for West or South or.., AA, WA, WW, WWW, etc...). Begins to be published in 1974. Ref. 1988A&AS...74..431V is a compilation. Catalogue is on electronic form, catalogue V/104/: (Nos 1-478) with missing numbers, some of these missing numbers being found in the literature. Nos up to 1107 are also found in the literature. See also [SBW2010] for the candidate jets of Smith, Bally & Walborn (2010MNRAS.405.1153S, table 3).
=E=	Catalogue in electronic form as V/104
Details on Acronym: HH
HH	(Smith+Bally+Walborn, 2010)
*****	Avoid the usage of HH, prefer [SBW2010]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HH77]
[HH77]	(Herbst+Havlen, 1977)
Write:	<<[HH77] NNN>>
N:	702
Object:	* in Assoc. (SIMBAD class: Star)
Note:	Identif. chart in Fig.1
in source:	NAME ASS ARA OB 1-
Ref:	=1977A&AS...30..279H
by	HERBST W. , HAVLEN R.J.
	Astron. Astrophys., Suppl. Ser., 30, 279-295 (1977)
	Ara OB1, NGC 6193 and Ara R1: an optical study of a very young southern complex.
o	Table 4: <[HH77] NNN> (Nos 1-702).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HH81]
[HH81]	(Ho+Haschick, 1981)
Write:	<<[HH81] GLL.l+B.b A>>
N:	8+5+3
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Components 'A' of 3 HII regions. These components could be interpreted as clusters of OB stars.
in source:	[WAM82] 010.62-0.38
in source:	[WAM82] 019.61-0.24
in source:	[WC89] 020.08-0.14
Ref:	=1981ApJ...248..622H
by	HO P.T.P. , HASCHICK A.D.
	Astrophys. J., 248, 622-637 (1981)
	Formation of OB clusters: VLA observations.
o	Table 1: <[HH81] G10.6-0.4 A> (Nos A-H), <[HH81] G19.6-0.2 A> (Nos A-E), <[HH81] G20.1-0.1 A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HH83]
[HH83]	(Haschick+Ho, 1983)
Write:	<<[HH83] AN>>
N:	8
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
in source:	W 33
Ref:	=1983ApJ...267..638H
by	HASCHICK A.D. , HO P.T.P.
	Astrophys. J., 267, 638-646 (1983)
	Formation of OB clusters : W 33 complex.
o	Table 1: <[HH83] AN> (Nos A, B1-B2, C-G)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HH86]
[HH86]	(Huang+Huang, 1986)= ([HH86a])
Write:	<<[HH86] HHMM+DDdA>>
N:	280
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Ref:	=1986Ap&SS.125...85H
by	HUANG K.-L. , HUANG J.-H.
	Astrophys. Space Sci., 125, 85-98 (1986)
	Optically selected QSO candidates in the field centered on selected Area 94.
o	Many misprints and errors
o	<[HH86] HHMM+DDdA> N=280
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HH86a]
[HH86a]	(Huang+Huang, 1986)
*****	Avoid the usage of [HH86a], prefer [HH86]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HH86b]
[HH86b]	(Henry Heasley, 1986)
Write:	<<[HH86b] GrG>>
N:	1
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	University of Hawaii 2.2m telescope observations. Study of the triple lens system PG 1115+08. Galaxies [YDG81] GN and [IFK98] GNN are members of a small group
Ref:	=1986Natur.321..139H
by	HENRY J.P. , HEASLEY J.N.
	Nature, 321, 139-142 (1986)
	High-resolution imaging from Mauna Kea : the triple quasar in 0.3-arcs seeing.
o	<[YDG81] GN> (No. 4) added. <[HH86b] GrG> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HH87]
[HH87]	(Hacking+Houck, 1987)
Write:	<<[HH87] NNN>> <<[HH87] N-NN>>
N:	141
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	IRAS Sky Survey. Table 5: 12 micro-m. detections: format '1-NN', (Nos 1-1 to 1-47) 25 micro-m. detections: format '2-NN', (Nos 2-1 to 2-37) 60 micro-m. detections: format '3-NN', (Nos 3-1 to 3-99) Table 6: final source list, (Nos 1-141)
Ref:	=1987ApJS...63..311H
by	HACKING P. , HOUCK J.R.
	Astrophys. J., Suppl. Ser., 63, 311-333 (1987)
	A very deep IRAS survey at l = 97, b = 30.
o	Table 5: <[HH87] N-NN> N=47+37+99, Table 6: <[HH87] NNN> (Nos 1-141)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HH92]
[HH92]	(Hughes+Hartigan, 1992)
Write:	<<[HH92] FNN>>
N:	34
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	In the format 'FNN', F stands for stars in the Field of Cha II DCld
in source:	NAME Cha II
Ref:	=1992AJ....104..680H
by	HUGHES J. , HARTIGAN P.
	Astron. J., 104, 680-690 (1992)
	Chamaeleon II: distance determination and HR diagram.
o	Table 1: (Nos F20-F90) misprint for (Nos F2-F9)
o	Tables 1, 2, 8: <[HH92] FNN> N=34
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HH95]
[HH95]	(Henden+Honeycutt, 1995)= ([HH97])
Write:	<<[HH95] AA CCC-NN>> <<[HH95] VNNNN CCC-NN>> <<[HH95] CCCN-NN>> <<[HH95] RX JHHMM+DD-NN>> <<[HH95] RE JHHMM+DD-NN>> <<[HH95] PG HHMM+DDd-NN>>
N:	619+2303
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Secondary photometric standards in the field of cataclysmic variables. Finding charts
Ref:	=1995PASP..107..324H
by	HENDEN A.A. , HONEYCUTT R.K.
	Publ. Astron. Soc. Pac., 107, 324-346 (1995)
	Secondary photometric standards for northern nova-like cataclysmic variables.
o	Designations 'CCC N' from Downes+Shara (1993, 1997) catalog of cataclysmic variables are not used in SIMBAD
o	Table 3: <[HH95] AA CCC-NN>, <[HH95] VNNNN CCC-NN>, <[HH95] CCCN-NN>, N=619
Ref:	=1997PASP..109..441H
by	HENDEN A.A. , HONEYCUTT R.K.
	Publ. Astron. Soc. Pac., 109, 441-460 (1997)
	Secondary photometric standards for northern cataclysmic variables and related objects.
o	Designations 'CCC N' from Downes+Shara (1993, 1997) catalog of cataclysmic variables are not used in SIMBAD
o	Table 3: <[HH95] AA CCC-NN>, <[HH95] VNNNN CCC-NN>, <[HH95] RX JHHMM+DD-NN>, <[HH95] RE JHHMM+DD-NN>, <[HH95] PG HHMM+DDd-NN> N=2303
=E=	Catalogue in electronic form as J/PASP/107/324
=E=	Catalogue in electronic form as J/PASP/109/441
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HH97]
[HH97]	(Henden+Honeycutt, 1997)
*****	Avoid the usage of [HH97], prefer [HH95]
Origin	of the Acronym: L (2007AJ....133.1934A)
Details on Acronym: [HH99]
[HH99]	(Holland+Hjorth, 1999)= ([HH99a])
Write:	<<[HH99] Knot N>>
N:	3
Object:	Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST STIS observations. Locations of possible star-forming regions near GRB 990123. Map in Fig.2. See also [BOD99].
Ref:	=1999A&A...344L..67H
by	HOLLAND S. , HJORTH J.
	Astron. Astrophys., 344, 67-70 (1999)
	Star-forming regions near GRB 990123.
o	Table 1: <[HH99] Knot N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HH99a]
[HH99a]	(Holland+Hjorth, 1999)
*****	Avoid the usage of [HH99a], prefer [HH99]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HH99b]
[HH99b]	(Hunter+Hoffman, 1999) (Not yet in Simbad)
Write:	<<[HH99b] DDO NN NN>> <<[HH99b] NGC NNNN N>> <<[HH99b] Haro NN N>> <<[HH99b] Mrk NNN N>> <<[HH99b] Zw 2335 N>>
N:	24
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Tables 1, 2: N=24 HII regions among the 189 studied. Table 5 give the number of observed HII in 67 galaxies.
Ref:	=1999AJ....117.2789H
by	HUNTER D.A. , HOFFMAN L.
	Astron. J., 117, 2789-2809 (1999)
	Emission-line spectroscopy of H II regions in irregular and blue compact dwarf galaxies.
o	T.6: [HG85] HII regions.
o	Tables 1, 2: <[HH99b] DDO NN NN>, <[HH99b] NGC NNNN N>, <[HH99b] Haro NN N>, <[HH99b] Mrk NNN N>, <[HH99b] Zw 2335 N>, N=24.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHA2003]
[HHA2003]	(Hall+Hutsemekers+Anderson+, 2005)
Write:	<<[HHA2003] QSO J0300+0048 abs N.NNNNNN>>
N:	1
Object:	Absorber
Note:	VLT UVES observations. Study of the spectra of SDSS J030000.56+004828.0 = QSO J0300+0048.
Ref:	=2003ApJ...593..189H
by	HALL P.B. , HUTSEMEKERS D., ANDERSON S.F., BRINKMANN J., FAN X., SCHNEIDER D.P., YORK D.G.
	Astrophys. J., 593, 189-202 (2003)
	VLT+UVES spectroscopy of the Ca II low-ionization broad absorption line quasar SDSS J030000.56+004828.0.
o	Text: <[HHA2003] QSO J0300+0048 abs N.NNNNNN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHA2012]
[HHA2012]	(HSU+HARTMANN+ALLEN+, 2012)
Write:	<<[HHA2012] NNN>>
N:	161 (SIMBAD class: YSO = Young Stellar Object)
Note:	MDM 2.4m Hiltner telescope OSMOS, MMT Hectospec, and Magellan Baade telescope IMACS observations of L 1641.
in source:	LDN 1641
Ref:	=2012ApJ...752...59H
by	HSU W.-H. , HARTMANN L., ALLEN L., HERNANDEZ J., MEGEATH S.T., MOSBY G., TOBIN J.J., ESPAILLAT C.
	Astrophys. J., 752, 59 (2012)
	The low-mass stellar population in L1641: evidence for environmental dependence of the stellar initial mass function.
o	Objects from tables 2 and 3 are designated under their 2MASS identification in SIMBAD, except object at 83.97163-06.93691 and object at 84.32064-06.65546, which are [FKV2013] 1294 and [FKV2013] 1335 respectively.
o	Table 4: <[HHA2012] NNN> N=161 among (Nos 6-861)
=E=	Catalogue in electronic form as <J/ApJ/752/59/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHB2004]
[HHB2004]	(Hutsemekers+Hall+Brinkmann, 2004)
Write:	<<[HHB2004] AN>> <<[HHB2004] QSO J0011+0055 abs N.NNNNN>>
N:	5+3
Object:	Absorber
Note:	Analysis of VLT+UVES spectra of the SDSS QSO J0011+0055. Detection of absorption systems, some are also designated as 'AN' in Table 1.
Ref:	=2004A&A...415...77H
by	HUTSEMEKERS D. , HALL P.B., BRINKMANN J.
	Astron. Astrophys., 415, 77-85 (2004)
	VLT + UVES spectroscopy of the low-ionization intrinsic absorber in SDSS J001130.56+005550.7.
o	(Erratum) Erratum vol. 422, p.509 (2004)
o	Table 1, text: <[HHB2004] QSO J0011+0055 abs N.NNNNN> N=5+3 = <[HHB2004] AN> (Nos A1-A3, B1-B2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHC2004]
[HHC2004]	(Healy+Hester+Claussen+, 2004)
Write:	<<[HHC2004] H2O M16 colN>> <<[HHC2004] H2O M16 colN A>> <<[HHC2004] H2O M16 NBay A>> <<[HHC2004] H2O M20 SE>> <<[HHC2004] H2O M20 TCN A>> <<[HHC2004] H2O NGC 2264>> <<[HHC2004] H2O S140 A>>
N:	16
Object:	H2O Maser (SIMBAD class: Maser)
Note:	Search for H2O masers emission associated with young low-mass protostars in HII regions with the VLA. When several components are found, a letter 'A' is added at the end of the format.
in source:	M 16 = Eagle Nebula = NGC 6611
in source:	M 20
in source:	NGC 2264
in source:	SH 2-140
Ref:	=2004ApJ...610..835H
by	HEALY K.R. , HESTER J.J., CLAUSSEN M.J.
	Astrophys. J., 610, 835-850 (2004)
	A very large array search for water masers in six H II regions: tracers of triggered low-mass star formation.
o	Text: <[PAB98] πN> (Nos π4, π5) added. Table 3: <[HHC2004] H2O M16 col2> N=1, <[HHC2004] H2O M16 col4> N=1, <[HHC2004] H2O M16 col5 A> (Nos A-C), <[HHC2004] H2O M16 NBay A> (Nos A-C), <[HHC2004] H2O M20 SE> N=1, <[HHC2004] H2O M20 TC3 A> (Nos A-C), <[HHC2004] H2O NGC 2264> N=1, <[HHC2004] H2O S140 A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHC2008]
[HHC2008]	(Hernandez Hartmann Calvet+, 2008)
Write:	<<[HHC2008] NNN>>
N:	579
Object:	*inCl (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC-MIPS and CTIO 0.9m telescope observations of the gam Vel Cluster. Use of 2MASS archival data.
in source:	NAME gam Vel Cluster
Ref:	=2008ApJ...686.1195H
by	HERNANDEZ J. , HARTMANN L., CALVET N., JEFFRIES R.D., GUTERMUTH R., MUZEROLLE J., STAUFFER J.
	Astrophys. J., 686, 1195-1208 (2008)
	A Spitzer view of protoplanetary disks in the γ Velorum cluster.
o	Table 1: <[HHC2008] NNN> (Nos 1-579).
=E=	Catalogue in electronic form as <J/ApJ/686/1195/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHC81]
[HHC81]	(Henry+Henriksen+Charles+, 1981)
Write:	<<[HHC81] GN>> <<[HHC81] A98W>>
N:	3+2
Object:	G in ClG + Subcluster of G (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	X-ray and optical observations of N=2 subclusters in ACO 98 and N=3 brightest galaxies in the northern subcluster.
in source:	ACO 98
Ref:	=1981ApJ...243L.137H
by	HENRY J.P. , HENRIKSEN M.J., CHARLES P.A., THORSTENSEN J.R.
	Astrophys. J., 243, 137-142 (1981)
	Observations of the two components of the Abell 98 cluster of galaxies.
o	Fig.1: <[HHC81] GN> (Nos G1-G3). Table 1: <[HHC81] A98W (Nos A98N-A98S).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHC93]
[HHC93]	(Hughes+Hartigan+Clampitt, 1993)
Write:	<<[HHC93] FFNN>>
N:	35
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	35 * in Lupus field. In the format: first digit 'A' is the letter F for Field, and second digit 'F' the field number (Nos 1-4), two last digits 'NN': running number in each field. The format is always a four digits format. Ex.: Object F409 is the star 9 in the field F4. No identif. charts.
in source:	NAME Lupus Cloud
Ref:	=1993AJ....105..571H
by	HUGHES J. , HARTIGAN P., CLAMPITT L.
	Astron. J., 105, 571-575 (1993)
	The distance to the Lupus star formation region.
o	<[HHC93] FNNN>, Lupus field *, N=35, Lupus I: format F1NN, Lupus II: F2NN, ...
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHC98]
[HHC98]	(Hannikainen+Hunstead+Campbell-Wilson+, 1998)
Write:	<<[HHC98] SN>>
N:	3
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	(Nos S1-S3), 3 reference sources in the field of GX 339-4
Ref:	=1998A&A...337..460H
by	HANNIKAINEN D.C. , HUNSTEAD R.W., CAMPBELL-WILSON D., SOOD R.K.
	Astron. Astrophys., 337, 460-464 (1998)
	MOST radio monitoring of GX 339-4.
o	Table 2: <[HHC98] SN> (Nos S1-S3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHD2006]
[HHD2006]	(Holmes+Hoette+Devore+, 2006)
Write:	<<[HHD2006] JHHMMSS.ss+DDMMSS.s>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxies of SN 2006BG, SN 2006BI, SN 2006BJ.
Ref:	=2006IAUC.8697....2H
by	HOLMES R. , HOETTE V., DEVORE H., MILLER P., MONARD L.A.G., QUIMBY R., ODEWAHN S.C., DEGLMAN F.
	IAU Circ., 8697, 2-None (2006)
	Supernovae 2006bg, 2006bh, 2006bi, 2006bj.
o	<[HHD2006] JHHMMSS.ss+DDMMSS.s> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHD2008]
[HHD2008]	(Haas+Heymann+Domke+, 2008)
Write:	<<[HHD2008] NW NNN>> <<[HHD2008] A NNNa>> <<[HHD2008] AN NNN>>
N:	3451
Object:	(Near IR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	CTIO 4m telescope ISPI NIR observations of several fields in the R CrA cloud.
in source:	NAME R CrA Cloud
Ref:	=2008A&A...488..987H
by	HAAS M. , HEYMANN F., DOMKE I., DRASS H., CHINI R., HOFFMEISTER V.
	Astron. Astrophys., 488, 987-996 (2008)
	A near-infrared survey of the entire R Coronae Australis cloud.
o	In the table A1, there are 2 objects designated as C 9, C 10, C 11, so we have added in the format a letter a and b to differentiate them.
o	Table A1: <[HHD2008] NW NNN> Nos among (Nos 1-628), <[HHD2008] AN NNNa> N=3451.
=E=	Catalogue in electronic form as J/A+A/488/987
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHD2009]
[HHD2009]	(Heller+Homeier+Dreizler+, 2009)
Write:	<<[HHD2009] SDSS JHHMM+DDMM>> <<[HHD2009] SDSS JHHMM+DDMM WD>> <<[HHD2009] SDSS JHHMM+DDMM M>>
N:	857+636+636
Object:	Binary * + WD + M * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=857 WD-M binaries from SDSS DR6.
Ref:	=2009A&A...496..191H
by	HELLER R. , HOMEIER D., DREIZLER S., OSTENSEN R.
	Astron. Astrophys., 496, 191-205 (2009)
	Spectral analysis of 636 white dwarf-M star binaries from the Sloan Digital Sky Survey.
o	Tables 1, 3: <[HHD2009] SDSS JHHMM+DDMM> N=857. Table 2: <[HHD2009] SDSS JHHMM+DDMM WD> N=636, <[HHD2009] SDSS JHHMM+DDMM M> N=636.
=E=	Catalogue in electronic form as J/A+A/496/191
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HHG
HHG	(Herbig-Haro Galaxy)
Write:	<<HHG LLL.l+BB.b>>
N:	1
Object:	Em. Obj. (SIMBAD class: EmObj = Emission Object)
Note:	See also CBSS.
Ref:	=1994MNRAS.267..871C
by	CAPPELLARO E. , BENETTI S., SABBADIN F., SALVADORI L., TURATTO M., ZANIN C.
	Mon. Not. R. Astron. Soc., 267, 871-880 (1994)
	New emission nebulae in the POSS field 18h 48m +0°.
o	Table 1: <HHG LLL.l+BB.b> N=1, <CBSS N> (Nos 1-3).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HHG
HHG	(Harris+Harris+Geisler)
*****	Avoid the usage of HHG, prefer [HHG2004]
Origin	of the Acronym: L (2006A&A...447..877G)
Details on Acronym: [HHG2004]
[HHG2004]	(Harris+Harris+Geisler, 2004)= (BTC) = (HHG)
Write:	<<[HHG2004] NNN>>
N:	327
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Note:	Big Throughput Camera (BTC) at the Cerro Tololo Inter-American observatory 4m telescope observations of the field around Cen A = NGC 5128. Study of the globular cluster system (GCS). See [HGH2004]
in source:	Cen A = NGC 5128
Ref:	=2004AJ....128..723H
by	HARRIS G.L.H. , HARRIS W.E., GEISLER D.
	Astron. J., 128, 723-735 (2004)
	Wide-field Washington photometry of the NGC 5128 globular cluster system. II. Large-scale properties of the system.
o	Table 4: <[HHG2004] NNN> (Nos 1-327).
=E=	Catalogue in electronic form as J/AJ/128/723
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHG86]
[HHG86]	(Henkel+Haschick+Gusten, 1986)
Write:	<<[HHG86] HHMMSS.s+DDMMSS>>
N:	19
Object:	Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=19 masers, among which 4 are new H2O masers.
Ref:	=1986A&A...165..197H
by	HENKEL C. , HASCHICK A.D., GUSTEN R.
	Astron. Astrophys., 165, 197-203 (1986)
	H2O maser emission from HH 6 and other star-forming regions.
o	Table 1: <[HHG86] HHMMSS.s+DDMMSS> N=19. Table 1: <[HMR80] H2O(D)> added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHG93]
[HHG93]	(Hunter+Hawley+Gallagher, 1993)
Write:	<<[HHG93] NGC NNNN NN>> <<[HHG93] IC NNNN N>> <<[HHG93] DDO NNN N>> <<[HHG93] NGC 1313 A>>
N:	85+1
Object:	Shell (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Table 3: N=85 filaments or shells or supershells in 23 galaxies. Maps in Figs 8-18. Fig.10: N=1 HII complex in NGC 1313, format 'A'. See also [HG90].
Ref:	=1993AJ....106.1797H
by	HUNTER D.A. , HAWLEY W.N., GALLAGHER III J.S.
	Astron. J., 106, 1797-1811 (1993)
	A survey for extra-H II region ionized gas structures in irregular galaxies.
o	Table 3: <[HHG93] NGC NNNN NN>, <[HHG93] IC NNNN N>, <[HHG93] DDO NNN N>, N=79. Fig.10: <[HHG93] NGC 1313 A> N=1.
Ref:	=2008MNRAS.383..864W
by	WESTMOQUETTE M.S. , SMITH L.J., GALLAGHER III J.S.
	Mon. Not. R. Astron. Soc., 383, 864-878 (2008)
	Studying the galactic outflow in NGC 1569.
o	Fig.2: <[HHG93] NGC 1569 NN> (Nos 14-20) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHG97]
[HHG97]	(Han+Hoessel+Gallagher+, 1997) (Not yet in Simbad)
Write:	<<[HHG97] a-NNNNN>> <<[HHG97] b-NNNNN>>
N:	78421+38203
Object:	* (SIMBAD class: Star)
Ref:	=1997AJ....113.1001H
by	HAN M. , HOESSEL J.G., GALLAGHER III J.S., HOLTZMAN J., STETSON P.B., TRAUGER J., BALLESTER G.E., BURROWS C., CLARKE J., CRISP D., GRIFFITHS R., GRILLMAIR C., HESTER J., KRIST J., MOULD J.R., SCOWEN P., STAPELFELDT K., WATSON A., WESTPHAL J.A.
	Astron. J., 113, 1001-1010 (1997)
	Stellar populations in the dwarf elliptical galaxy NGC 147.
o	Table 2(a): <[HHG97] a-NNNNN> N=78421. Table 2(b): <[HHG97] b-NNNNN> N=38203
=E=	Catalogue in electronic form as J/AJ/113/1001
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHH2005]
[HHH2005]	(Hasjimoto+Henry+Hasinger+, 2005)
Write:	<<[HHH2005] N>>
N:	6
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Subaru Suprime-Cam and Keck-DEIMOS spectroscopic observations of galaxies in the cluster RX J1053.7+5735.
in source:	RX J1053.0+5735
Ref:	=2005A&A...439...29H
by	HASHIMOTO Y. , HENRY J.P., HASINGER G., SZOKOLY G., SCHMIDT M.
	Astron. Astrophys., 439, 29-33 (2005)
	Galaxy populations of double cluster RX J1053.7+5735 at z=1.13.
o	Fig.1, Table 1: <[HHH2005] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HHH86
HHH86	(Hesser+Harris+Harris, 1986)
*****	Avoid the usage of HHH86, prefer [VHH81]
Origin	of the Acronym: L (2004ApJS..150..367P)
Details on Acronym: [HHH98]
[HHH98]	(Hughes+Han+Hoessel+, 1998)
Write:	<<[HHH98] RNN>> <<[HHH98] VNN>>
N:	31+13
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations. Table 2: (Nos R1-R31), reference stars. Table 6: (Nos V1-V13), Cepheids in NGC 7331.
in source:	NGC 7331
Ref:	=1998ApJ...501...32H
by	HUGHES S.M.G. , HAN M., HOESSEL J., FREEDMAN W.L., KENNICUTT R.C., MOULD J.R., SAHA A., STETSON P.B., MADORE B.F., SILBERMANN N.A., HARDING P., FERRARESE L., FORD H., GIBSON B.K., GRAHAM J.A., HILL R., HUCHRA J., ILLINGWORTH G.D., PHELPS R., SAKAI S.
	Astrophys. J., 501, 32-53 (1998)
	The Hubble space telescope extragalactic distance scale key project. X. The cepheid distance to NGC 7331.
o	Table 2: <[HHH98] RNN> (Nos R1-R31). Table 6: <[HHH98] VNN> (Nos V1-V13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HHIC
HHIC	(Homogeneized Hydrogen I Catalog)
**	catalog: use LEDA
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HHJ2008]
[HHJ2008]	(Harvey+Huard+Jorgensen+, 2008)
Write:	<<[HHJ2008] NNN>>
N:	202
Object:	Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC and MIPS observations of N=202 YSO candidates in the field of IC5146.
in source:	Gould Belt:IC 5146 = IC 5146
Ref:	=2008ApJ...680..495H
by	HARVEY P.M. , HUARD T.L., JORGENSEN J.K., GUTERMUTH R.A., MAMAJEK E.E., BOURKE T.L., MERIN B., CIEZA L., BROOKE T., CHAPMAN N., ALCALA J.M., ALLEN L.E., EVANS II N.J., DI FRANCESCO J., KIRK J.M.
	Astrophys. J., 680, 495-516 (2008)
	The Spitzer survey of interstellar clouds in the Gould belt. I. IC 5146 observed with IRAC and MIPS.
o	Tables 5, 6, 7, col(1): <[HHJ2008] NNN> (Nos 1-202). Tables 5, 6, 7, 9, col(2): <SSTgbs JHHMMSSss+DDMMSSs> N=202+678.
=E=	Catalogue in electronic form as J/ApJ/680/495
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHK2012]
[HHK2012]	(HSIEH+HO+KOHNO+, 2012)
Write:	<<[HHK2012] N>>
N:	8
Object:	Giant molecular cloud association (GMA) (SIMBAD class: MolCld = Molecular Cloud)
Note:	SMA 12CO(3-2), HCN, and HCO+ observations of the circumnuclear region of NGC 1097.
Ref:	=2012ApJ...747...90H
by	HSIEH P.-Y. , HO P.T.P., KOHNO K., HWANG C.-Y., MATSUSHITA S.
	Astrophys. J., 747, 90 (2012)
	Probing circumnuclear environments with the HCN(J = 3-2) and HCO^+(J = 3-2) lines: case of NGC 1097.
o	Table 1: <[HHK2012] N> N=8 (Nos 1-8)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HHL
HHL	(Herbig Haro Like obj.)
Write:	<<HHL NNa>>
N:	77+11
Object:	HH-like (SIMBAD class: ISM = Interstellar Medium Object)
Stat:	is completely incorporated in Simbad
Ref:	=1987RMxAA..15...53G
by	GYULBUDAGHIAN A.L. , RODRIGUEZ L.F., MENDOZA-TORRES E.
	Rev. Mex. Astron. Astrofis., 15, 53-57 (1987)
	Three new H2O masers located near Herbig-Haro-like nebulosities.
o	<HHL NN> (Nos 1-77)
Ref:	=1998Ap.....41..382G
by	GYULBUDAGHIAN A.L.
	Astrophysics, 41, 382-391 (1998)
	Nonsteady objects associated with star-forming regions. Relationship to stellar associations, infrared sources, and water masers.
o	Cross-id.: G1-NN = [G82a] in table 1, [G82b] in table 2. G2-NN = [G82c] in table 1, [G84b] in table 2. G3-NN = [G84d] 1-N in table 1, [G84c] in table 2. Both designations 'G4' have not been identified (ref. not found). GM 1-NN = GM 1-NN but GM 2-NN = GM 3-NN in SIMBAD.
o	Table 1: <[G98] NNN> (Nos 1-189). Table 2: <HHL NNa> N=11.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HHL2001]
[HHL2001]	(Hotzel+Harju+Lemke+, 2001)
Write:	<<[HHL2001] B217WW>>
N:	3
Object:	Core (SIMBAD class: PartofCloud = Part of Cloud)
Note:	N=3 cores of dense gas in Barnard 217.
in source:	Barnard 217
Ref:	=2001A&A...372..302H
by	HOTZEL S. , HARJU J., LEMKE D., MATTILA K., WALMSLEY C.M.
	Astron. Astrophys., 372, 302-316 (2001)
	Dense gas and cold dust in the dark core B217.
o	Text, table 1: <[HHL2001] B217WW> (Nos SW, NE, NW).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHL2006]
[HHL2006]	(Harju+Haikala+Lehtinen+, 2009)
Write:	<<[HHL2006] OriB9 W>>
N:	2
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	APEX observations of the massive, cold core OriB9.
in source:	[CM95] Ori B9
Ref:	=2006A&A...454L..55H
by	HARJU J. , HAIKALA L.K., LEHTINEN K., JUVELA M., MATTILA K., MIETTINEN O., DUMKE M., GUESTEN R., NYMAN L.-A.
	Astron. Astrophys., 454, 55-58 (2006)
	Detection of H_{2}D^+ in a massive prestellar core in Orion B.
o	Table 1: <[HHL2006] OriB9 W> (Nos OriB9 E, OriB9 N).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHL2012]
[HHL2012]	(Huynh+Hopkins+Lenc+, 2015) (Not yet in Simbad)
Write:	<<[HHL2012] NNN>> <<[HHL2012] NNNa>>
N:	123+29
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ATCA 5.5GHz observations of N=123 sources (format NNN) and N=29 multiple component sources (format NNNa) in the extended Chandra Deep Field South, by the Australia Telescope Large Area Survey (ATLAS) team. See also ATCDFS5, [HBH2015b], as well as ATCDFS9, [HSN2020].
in source:	NAME ECDFS
Ref:	=2012MNRAS.426.2342H
by	HUYNH M.T. , HOPKINS A.M., LENC E., MAO M.Y., MIDDELBERG E., NORRIS R.P., RANDALL K.E.
	Mon. Not. R. Astron. Soc., 426, 2342-2358 (2012)
	The ATLAS 5.5 GHz survey of the extended Chandra Deep Field South: catalogue, source counts and spectral indices.
o	Table 1, col(1): <[HHL2012] NNN> N=123 among (Nos 1-145), <[HHL2012] NNNA> N=29 among (Nos 31a-31c to 138a-138c). Table 1, col(2): <ATCDFS5 JHHMMSS.ss+DDMMSS.s> N=142.
=E=	Catalogue in electronic form as <J/MNRAS/426/2342/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHL82]
[HHL82]	(Hintzen+Hill+Lindley+, 1982)
Write:	<<[HHL82] ANNNN NNN>>
N:	20+51+17+12
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Table 1: Galaxies in 4 ACO clusters. Finding charts in figs.(2a-2e)
in source:	ACO 400
in source:	ACO 576
in source:	ACO 1767
in source:	ACO 2124
Ref:	=1982AJ.....87.1656H
by	HINTZEN P. , HILL J.M., LINDLEY D., SCOTT J.S., ANGEL J.R.P.
	Astron. J., 87, 1656-1667 (1982)
	Medusa spectroscopy of A400, A576, A1767, and A2124.
o	Table 1: <[HHL82] A400 NNN> N=20 among (Nos 203-329), <[HHL82] A576 NNN> N=51 among (Nos 201-287), <[HHL82] A1767 NNN> N=17 among (Nos 201-262), <[HHL82] A2124 NNN> N=12 among (Nos 201-237).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HHM
HHM	(Hanes+Harris+Madore) (Not yet in Simbad)
*****	Avoid the usage of HHM, prefer [HHM76]
Origin	of the Acronym: L (1984MNRAS.209..169K)
Details on Acronym: HHM
HHM	(Harris+Harris+McLaughlin)
*****	Avoid the usage of HHM, prefer [HHM98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HHM2005]
[HHM2005]	(Haikala+Harju+Mattila+, 2005)
Write:	<<[HHM2005] NN>>
N:	71
Object:	C18O Clump (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	SEST C18O observations of N=71 clumps in the Cha I cloud.
in source:	NAME Cha I
Ref:	=2005A&A...431..149H
by	HAIKALA L.K. , HARJU J., MATTILA K., TORISEVA M.
	Astron. Astrophys., 431, 149-163 (2005)
	Clumpy filaments of the Chamaeleon I cloud: C^{18}O mapping with the SEST.
o	Fig.1, Table 1: <[HHM2005] NN> (Nos 1-71).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHM2006]
[HHM2006]	(Higdon+Higdon+Marshall, 2006)
Write:	<<[HHM2006] NNa>>
N:	75+2
Object:	(Mid IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC observations of the fields of the 2 tidal galaxies [BDL2001] NGC 5291N and [BDL2001] NGC 5291S.
Ref:	=2006ApJ...640..768H
by	HIGDON S.J. , HIGDON J.L., MARSHALL J.
	Astrophys. J., 640, 768-783 (2006)
	First detection of PAHs and warm molecular hydrogen in tidal dwarf galaxies.
o	NGC 5291N and S = [BDL2001] NGC 5291N and [BDL2001] NGC 5291S.
o	Table 4: <[HHM2006] NN> (Nos 1-75). Fig.12: <[HHM2006] NNa> (Nos 12a, 48a).
=E=	Catalogue in electronic form as J/ApJ/640/768
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHM2007]
[HHM2007]	(Hernandez+Hartmann+Megeath+, 2007)= (SO)
Write:	<<[HHM2007] NNNN>>
N:	336+133
Object:	* in Cl* (SIMBAD class: Star)
Note:	Spitzer MIPS observations of the sig Ori Cluster. See also [HRB2007].
in source:	NAME sig Ori Cluster
Ref:	=2007ApJ...662.1067H
by	HERNANDEZ J. , HARTMANN L., MEGEATH T., GUTERMUTH R., MUZEROLLE J., CALVET N., VIVAS A.K., BRICENO C., ALLEN L., STAUFFER J., YOUNG E., FAZIO G.
	Astrophys. J., 662, 1067-1081 (2007)
	A Spitzer Space Telescope study of disks in the young σ Orionis cluster.
o	Tables 1, 2: <[HHM2007] NNNN> N=336+133 among (Nos 9-1375).
=E=	Catalogue in electronic form as J/ApJ/662/1067
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHM2010]
[HHM2010]	(Hammer+Hornschemeier+Mobasher+, 2010)
Write:	<<[HHM2010] DDD.ddddd+DD.ddddd>>
N:	9700
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	GALEX observations of the Coma Cluster. Use of SDSS data.
in source:	Coma Cluster = ACO 1656
Ref:	=2010ApJS..190...43H
by	HAMMER D. , HORNSCHEMEIER A.E., MOBASHER B., MILLER N., SMITH R., ARNOUTS S., MILLIARD B., JENKINS L.
	Astrophys. J., Suppl. Ser., 190, 43-57 (2010)
	Deep GALEX observations of the Coma cluster: source catalog and galaxy counts.
o	Table 1: <[HHM2010] DDD.ddddd+DD.ddddd> N=9700.
=E=	Catalogue in electronic form as J/ApJS/190/43
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHM76]
[HHM76]	(Hanes+Harris+Madore, 1976)= (HHM) (Not yet in Simbad)
Write:	<<[HHM76] NGC NNNN NN>> <<[HHM76] NGC NNNN-NNNN NN>> <<[HHM76] NGC NNNN-NNNN-NNNN NN>>
N:	155
Object:	* (SIMBAD class: Star)
Note:	UBV photometry for 155 stars in 16 'NGC' sequences. Finding charts in Plates 5-9.
Ref:	=1976MNRAS.177..653H
by	HANES D.A. , HARRIS W.E., MADORE B.F.
	Mon. Not. R. Astron. Soc., 177, 653-659 (1976)
	UBV sequences for selected Virgo galaxies.
o	Table II: <[HHM76] NGC NNNN NN>, <[HHM76] NGC NNNN-NNNN NN>, <[HHM76] NGC NNNN-NNNN-NNNN NN>, N=155.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHM93]
[HHM93]	(Harju+Haikala+Mattila+, 1993)
Write:	<<[HHM93] AN>>
N:	4+3
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Note:	Figs 1, 2, Table 1: N=4 condensations (or clumps, or cores) in R CrA cloud core, (Nos A-D). N=3 sub-condensations (Nos A1-A3).
in source:	NAME R CrA Cloud
Ref:	=1993A&A...278..569H
by	HARJU J. , HAIKALA L.K., MATTILA K., MAUERSBERGER R., BOOTH R.S., NORDH H.L.
	Astron. Astrophys., 278, 569-583 (1993)
	Large scale structure of the R Coronae Australis cloud core.
o	NE and SW jaws not in SIMBAD.
o	Figs 1, 2, Table 1: <[HHM93] A> (Nos A-D), <[HHM93] AN> (Nos A1-A3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHM94]
[HHM94]	(Hayward+Houck+Miles, 1994)= (SC)
Write:	<<[HHM94] NN>>
N:	13
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	NAME Trapezium Nebula
Ref:	=1994ApJ...433..157H
by	HAYWARD T.L. , HOUCK J.R., MILES J.W.
	Astrophys. J., 433, 157-163 (1994)
	Thermal infrared imaging of subarcsecond structure in the Trapezium Nebula.
o	<[HHM94] NN> N=13
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHM97]
[HHM97]	(Heisler+Hill+McCall+, 1997)
Write:	<<[HHM97] NN>>
Object:	* + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Identif. chart in Fig.1
in source:	NAME SDIG
Ref:	=1997MNRAS.285..374H
by	HEISLER C.A. , HILL T.L., McCALL M.L., HUNSTEAD R.W.
	Mon. Not. R. Astron. Soc., 285, 374-386 (1997)
	The Sculptor dwarf irregular galaxy SDIG: present and past.
o	Table 4: <[HHM97] NN> (Nos 1-34)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHM98]
[HHM98]	(Harris+Harris+McLaughlin, 1998)= (HHM)
Write:	<<[HHM98] +xx.xx+yyy.yy>>
N:	80
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Note:	Table 2: partial listing of data for the brightest objects.
in source:	M 87 = NGC 4486 = Virgo A
Ref:	=1998AJ....115.1801H
by	HARRIS W.E. , HARRIS G.L.H., McLAUGHLIN D.E.
	Astron. J., 115, 1801-1822 (1998)
	M87, globular clusters, and galactic winds: issues in giant galaxy formation.
o	Table 2: <[HHM98] +xx.xx+yyy.yy> N=80.
=E=	Catalogue in electronic form as J/AJ/115/1801
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHO88]
[HHO88]	(Hill+Hintzen+Oegerle+, 1988)
Write:	<<[HHO88] NN>>
N:	40
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Spectrographic observations on the Steward Observatory 2.3m telescope of ACO 1795. See also [HO93] table 5.
in source:	ACO 1795
Ref:	=1988ApJ...332L..23H
by	HILL J.M. , HINTZEN P., OEGERLE W.R., ROMANISHIN W., LESSER M.P., EISENHAMER J.D., BATUSKI D.J.
	Astrophys. J., 332, 23-27 (1988)
	Peculiar velocities of cD galaxies: MX spectroscopy of Abell 1795.
o	Table 1, Fig.1: <[HHO88] NN> N=40 among (Nos 1-87).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHP90]
[HHP90]	(Huchra+Henry+Postman+, 1990)
Write:	<<[HHP90] HHMM+DDMMA>>
N:	352
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=352 G in 145 ACO ClG
Ref:	=1990ApJ...365...66H
by	HUCHRA J.P. , HENRY J.P., POSTMAN M., GELLER M.J.
	Astrophys. J., 365, 66-85 (1990)
	A deep Abell cluster redshift survey.
o	p. 73, error: '[HHP90] 1059+5859' (not 1059+1410)
o	Table 2: <[HHP90] HHMM+DDMMA> N=352
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHP98]
[HHP98]	(Hoff+Henning+Pfau, 1998)= (TW HyaX) = (CoD-29 8887X)
Write:	<<[HHP98] TW Hya XNNA>> <<[HHP98] CoD-29 8887 XNNA>>
N:	58+49+13
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations. Table 2: N=58 X-ray sources around TW Hya. Table 3: N=49 X-ray sources around CoD -29 8887. Table 4: Optical counterparts of the X-ray sources: a letter 'A' is added at the end of the format when there are several possibilities of optical counterpart for the same X-ray source. (The authors used this rule only for one source, but it is used systematically in SIMBAD)
Ref:	=1998A&A...336..242H
by	HOFF W. , HENNING T., PFAU W.
	Astron. Astrophys., 336, 242-250 (1998)
	The nature of isolated T Tauri stars.
o	Table 2: <[HHP98] TW Hya XNN> (Nos X1-X58). Table 3: <[HHP98] CoD-29 8887 XNN> (Nos X1-X49). Table 4: <[HHP98] TW Hya XNNA> N=9, <[HHP98] CoD-29 8887 XNNA> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHR2009]
[HHR2009]	(Hill+Haffner+Reynolds, 2009) (Not yet in Simbad)
Write:	<<[HHR2009] Clump A>> <<[HHR2009] Tip>> <<[HHR2009] Tail>>
N:	4
Object:	Clump (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Wisconsin H-Alpha Mapper (WHAM) observations of ionized gas in the Smith Cloud.
in source:	NAME Smith Cloud
Ref:	=2009ApJ...703.1832H
by	HILL A.S. , HAFFNER L.M., REYNOLDS R.J.
	Astrophys. J., 703, 1832-1838 (2009)
	Ionized gas in the Smith Cloud.
o	Fig. 3, Table 2: <[HHR2009] Clump A> (Nos A-B), <[HHR2009] Tip> N=1, <[HHR2009] Tail> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHR2012]
[HHR2012]	(Haas+Hackstein+Ramolla+, 2012)= (GDS)
Write:	<<[HHR2012] DDD.dddddd+DD.dddddd>>
N:	∼2200
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Observations of N∼2200 variable stars, using a robotic 15-cm twin telescope of the Universitätsternwarte Bochum near Cerro Armazones in Chile, as part of the Bochum Galactic Disk survey (GDS). See also [HFH2015].
Ref:	=2012AN....333..706H
by	HAAS M. , HACKSTEIN M., RAMOLLA M., DRASS H., WATERMANN R., LEMKE R., CHINI R.
	AN, 333, 706-716 (2012)
	The Bochum survey of the southern Galactic disk: I. Survey design and first results on 50 square ° monitored in 2011.
o	Table 2: <[HHR2012] DDD.dddddd+DD.dddddd> N~2200.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHS2008]
[HHS2008]	(Halkola+Hildebrandt+Schrabback+, 2008)
Write:	<<[HHS2008] NNa>>
N:	30
Object:	G (SIMBAD class: GravLens_Candidate = Gravitational Lens Candidate)
Stat:	is completely incorporated in Simbad
Note:	HST-ACS images of the ClG J1347-1145.
in source:	ClG J1347-1145 = RX J1347.5-1145
Ref:	=2008A&A...481...65H
by	HALKOLA A. , HILDEBRANDT H., SCHRABBACK T., LOMBARDI M., BRADAC M., ERBEN T., SCHNEIDER P., WUTTKE D.
	Astron. Astrophys., 481, 65-77 (2008)
	The mass distribution of RX J1347-1145 from strong lensing.
o	Table A1, Figs 2, A: <[HHS2008] NNa> N=30.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHS2010]
[HHS2010]	(Hoshino+Henry+Sato+, 2010)
Write:	<<[HHS2010] NN>>
N:	15
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Suzaku XIS X-ray observations of the northern outskirts of the galaxy cluster Abell 1413. Use of XMM-Newton images.
in source:	ACO 1413
Ref:	=2010PASJ...62..371H
by	HOSHINO A. , HENRY J.P., SATO K., AKAMATSU H., YOKOTA W., SASAKI S., ISHISAKI Y., OHASHI T., BAUTZ M., FUKAZAWA Y., KAWANO N., FURUZAWA A., HAYASHIDA K., TAWA N., HUGHES J.P., KOKUBUN M., TAMURA T.
	PASJ, 62, 371-389 (2010)
	X-ray temperature and mass measurements to the virial radius of Abell 1413 with Suzaku.
o	Table 2: <[HHS2010] NN> (Nos 1-15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHS2014]
[HHS2014]	(Higdon+Higdon+Smith+, 2014)
Write:	<<[HHS2014] {Arp}NNN {S\|N\|E}N>> <<[HHS2014] ArpNNN SWN>> <<[HHS2014] SQ A>> <<[HHS2014] NGC5291 NN>> <<[HHS2014] NGC NNN>> (not recognised by Simbad, but found in literature) <<[HHS2014] Arp NNN>>
N:	67 (SIMBAD class: Infrared = Infra-Red Source)
Note:	Spitzer IRAC observation of N=67 intergalactic star-forming objects (ISFOs).
Ref:	=2014ApJ...787..103H
by	HIGDON S.J.U. , HIGDON J.L., SMITH B.J., HANCOCK M.
	Astrophys. J., 787, 103 (2014)
	Star formation And the Interstellar medium in Nearby Tidal Streams (SAINTS): Spitzer mid-infrared spectroscopy and imaging of intergalactic star-forming objects.
o	Table 1: <[HHS2014] ArpNNN AN> N=38, <[HHS2014] Arp107 SW1> N=1, <[HHS2014] Arp284 AAN> N=2 (Nos SW1 to SW2), <[HHS2014] SQ A> N=2 (Nos A and B), <[HHS2014] NGC5291 NN> N=24 (Nos 13 to 51).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHS2020]
[HHS2020]	(Herenz+Hayes+Scarlata, 2020)
Write:	<<[HHS2020] LAE N>>
N:	4
Object:	LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	VLT MUSE observations of N=4 Lymanα emitters (LAEs) in the Lymanα blob [TSK2001] LAB 1.
in source:	[TSK2001] LAB 1 = [MYH2004] LAB 1
Ref:	=2020A&A...642A..55H
by	HERENZ E.C. , HAYES M., SCARLATA C.
	Astron. Astrophys., 642A, 55-55 (2020)
	Deciphering the Lyman α blob 1 with deep MUSE observations.
o	Fig. 4, Table 3: <[HHS2020] LAE N> (Nos LAE 1-LAE 4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHS87]
[HHS87]	(Harvey+Hyland+Straw, 1987)= (IRS)
Write:	<<[HHS87] IRS NN>>
N:	57
Object:	(near IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	NGC 6334:MFSW IV = MFSW IV
Ref:	=1987ApJ...317..173H
by	HARVEY P.M. , HYLAND A.R., STRAW S.M.
	Astrophys. J., 317, 173-179 (1987)
	A near-infrared study of the NGC 6334-IV region.
o	cross-id. HG = [HG83] IRS-IV-N, PF = [PF82] NGC 6334A IRS N
o	Table 1: <[HHS87] IRS NN> (Nos 1-57)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHS94]
[HHS94]	(Hill+Home+Smith+, 1994)
Write:	<<[HHS94] NN>>
N:	22
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	See also [HFS98].
in source:	NGC 4449
Ref:	=1994ApJ...430..568H
by	HILL R.S. , HOME A.T., SMITH A.M., BRUHWEILER F.C., CHENG K.P., HINTZEN P.M.N., OLIVERSEN R.J.
	Astrophys. J., 430, 568-580 (1994)
	Star formation in NGC 4449: MAMA-detector UV imagery and Fabry-Perot Balmer-line imagery.
o	<[HHS94] NN> N=22
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHT2009]
[HHT2009]	(Hutton+Henden+Terrell, 2009)
Write:	<<[HHT2009] NN>>
N:	9
Object:	* (SIMBAD class: Star)
Note:	Comparison stars in the field of CX Cep. SRO 0.35m robotic telescope observations.
Ref:	=2009PASP..121..708H
by	HUTTON K. , HENDEN A., TERRELL D.
	PASP, 121, 708-715 (2009)
	Photometry of the CX Cephei system (WR 151).
o	Table 1: <[HHT2009] NN> N=9 among (Nos 2-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHT2010]
[HHT2010]	(Hiramatsu+Hirano+Takakuwa, 2010) (Not yet in Simbad)
Write:	<<[HHT2010] SMM 2 WN>>
N:	4
Object:	Outflow (SIMBAD class: Outflow)
Note:	Nobeyama 45m telescope observations of Barnard 1.
in source:	Barnard 1
Ref:	=2010ApJ...712..778H
by	HIRAMATSU M. , HIRANO N., TAKAKUWA S.
	Astrophys. J., 712, 778-789 (2010)
	Outflow-core interaction in Barnard 1.
o	Fig. 6, Table 6: <[HHT2010] SMM2 WN> (Nos W1-W3, E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHT2016]
[HHT2016]	(Hoag+Huang+Treu+, 2016)
Write:	<<[HHT2016] NNN.N>>
N:	243
Object:	Poss. Grav. lensed image (SIMBAD class: LensedImage_Candidate = Gravitationally Lensed Image Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=252 gravitationally lensed image candidates in the field of the galaxy cluster MCS J0416.1-2403. Use of GLASS, Hubble Frontier Fields (HFF), and CLASH data. See also [JCL2014], [JSB2014], [RJL2014], [ZFM2015].
in source:	MCS J0416.1-2403
Ref:	=2016ApJ...831..182H
by	HOAG A. , HUANG K.-H., TREU T., BRADAC M., SCHMIDT K.B., WANG X., BRAMMER G.B., BROUSSARD A., AMORIN R., CASTELLANO M., FONTANA A., MERLIN E., SCHRABBACK T., TRENTI M., VULCANI B.
	Astrophys. J., 831, 182-182 (2016)
	The Grism Lens-Amplified Survey from Space (GLASS). VI. Comparing the mass and light in MACS J0416.1-2403 using Frontier Field imaging and GLASS spectroscopy.
o	Table 2: <[HHT2016] NNN.N> N=243 among (Nos 1.1-1.3 to 207.1-207.2).
=E=	Catalogue in electronic form as <J/ApJ/831/182/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHV2005]
[HHV2005]	(Hamilton+Herbst+vRBA+ 2005) (Not yet in Simbad)
Write:	<<[HHV2005] A>>
N:	7
Object:	* (SIMBAD class: Star)
Note:	Comparison stars in the field of the star Cl* NGC 2264 VVO 15D.
Ref:	=2005AJ....130.1896H
by	HAMILTON C.M. , HERBST W., VRBA F.J., IBRAHIMOV M.A., MUNDT R., BAILER-JONES C.A.L., FILIPPENKO A.V., LI W., BEJAR V.J.S., ABRAHAM P., KUN M., MOOR A., BENKO J., CSIZMADIA S., DEPOY D.L., POGGE R.W., MARSHALL J.L.
	Astron. J., 130, 1896-1915 (2005)
	The disappearing act of KH 15D: photometric results from 1995 to 2004.
o	Fig.1, Table 3: <[HHV2005] A> (Nos A-G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHW2005]
[HHW2005]	(Higdon+Higdon+Weedman+, 2005)
Write:	<<[HHW2005] NNN>>
N:	36
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA deep 20cm observations within the Bootes field. Cross-identification with the NOAO deep wide-field survey (NDWFS), Spitzer MIPS, and deep Chandra observations.
Ref:	=2005ApJ...626...58H
by	HIGDON J.L. , HIGDON S.J.U., WEEDMAN D.W., HOUCK J.R., LE FLOC'H E., BROWN M.J.I., DEY A., JANNUZI B.T., SOIFER B.T., RIEKE M.J.
	Astrophys. J., 626, 58-69 (2005)
	Spitzer observations of optically ``Invisible'' radio and X-ray sources: high-redshift active galactic nuclei.
o	Table 2: <[HHW2005] NNN> N=36 among (Nos 9-441).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HHW91]
[HHW91]	(Hamilton+Helfand+Wu, 1991)
Write:	<<[HHW91] HHMMSS.ss+DDMMSS.ss>>
N:	33
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Reanalysis of Einstein Observatory Deep Survey data.
Ref:	=1991ApJ...379..576H
by	HAMILTON T.T. , HELFAND D.J., WU X.
	Astrophys. J., 379, 576-585 (1991)
	Faint X-ray source counts and the origin of the X-ray background.
o	Table 2: <[HHW91] HHMMSS.ss+DDMMSS.ss> N=33
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Hi2000
Hi2000	(Hirano+)
*****	Avoid the usage of Hi2000, prefer [HMU2001]
Origin	of the Acronym: L (2001A	A...375..40C)
Details on Acronym: [HI2001]
[HI2001]	(Hinkley +Im+, 2001)
Write:	<<[HI2001] GSSFFN-xxyy>>
N:	5
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Sample of 5 early-type galaxies, utilizing HST NIR camera and MOS with WFPC2. In the format 'GSS' stands for Groth Strip Survey, see DEEP-GSS.
Ref:	=2001ApJ...560L..41H
by	HINKLEY S. , IM M.
	Astrophys. J., 560, 41-44 (2001)
	Optical-near-infrared color gradients in early-type galaxies at z≤1.0.
o	SSA 13 55 = [CSH96] SSA 13 55 in SIMBAD.
o	Table 1, Fig.1: <[HI2001] GSSFFC-xxyy> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HI86]
[HI86]	(He+Impey, 1986)
Write:	<<[HI86] EGN>> <<[HI86] OEGN>> <<[HI86] HIIN>>
N:	10
Object:	EmG (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=5 emission-line galaxies and N=5 other candidates in the Virgo region.
Ref:	=1986MNRAS.221..727H
by	HE X.-T. , IMPEY C.D.
	Mon. Not. R. Astron. Soc., 221, 727-737 (1986)
	Emission-line galaxies in the Virgo region.
o	Tables 1, 2: <[HI86] EGN> (Nos EG1-EG7), <[HI86] OEGN> (Nos OEG1-OEG2), <[HI86] HIIN> (No. 2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HIB95]
[HIB95]	(Hill+Isensee+Bohlin+, 1995)
Write:	<<[HIB95] NNN-NNN>>
N:	611
Object:	(UV) (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	UIT aboard Astro-1 Spacelab mission. Table 4: In the format 'NNN-NNN', the first left 'NNN' stands for the '[V64] NNN' OB associations in which sources are found.
in source:	M 31 = NGC 224
Ref:	=1995ApJS...98..595H
by	HILL J.K. , ISENSEE J.E., BOHLIN R.C., CHENG K.P., HINTZEN P.M.N., O'CONNELL R.W., ROBERTS M.S., SMITH A.M., SMITH E.P., STECHER T.P.
	Astrophys. J., Suppl. Ser., 98, 595-615 (1995)
	Ultraviolet and optical observations of OB associations in M31.
o	cross-id.: MAC = [MAC86] 1-, M = [MLV92], Bo = Bol, CNNN = [H81] B-NNN
o	Table 4: <[HIB95] NNN-NNN> N=611
=E=	Catalogue in electronic form as J/ApJS/98/595
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HIC
HIC	(Hipparcos Input Catalogue)= (INCA)
Write:	<<HIC NNNNNN>>
N:	120313
Object:	* (SIMBAD class: Star)
Ref:	=1992BICDS..41....9T
by	TURON C. , CREZE M., EGRET D., GOMEZ A., GRENON M., JAHREISS H., REQUIEME Y., ARGUE A.N., BEC-BORSENBERGER A., DOMMANGET J., MENNESSIER M.O., ARENOU F., CHARETON M., CRIFO F., MERMILLIOD J.C., MORIN D., NICOLET B., NYS O., PREVOT L., ROUSSEAU M., PERRYMAN M.A.C.
	Bull. Inf. Centre Donnees Stellaires, 41, 9-20 (1992)
	The Hipparcos Input Catalogue.
o	<HIC NNNNNN> N=120313.
Ref:	=1993BICDS..43....5T
by	TURON C. , CREZE M., EGRET D., GOMEZ A., GRENON M., JAHREISS H., REQUIEME Y., ARGUE A.N., BEC-BORSENBERGER A., DOMMANGET J., MENNESSIER M.O., ARENOU F., CHARETON M., CRIFO F., MERMILLIOD J.C., MORIN D., NICOLET B., NYS O., PREVOT L., ROUSSEAU M., PERRYMAN M.A.C.
	Bull. Inf. Centre Donnees Stellaires, 43, 5-None (1993)
	Version 2 of the Hipparcos Input Catalogue.
o	<HIC NNNNNN> N=120313.
=E=	Catalogue in electronic form as I/196
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HIC
HIC	(Hydrogen I Catalog)
**	catalog: use LEDA
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Hick
Hick	(Hickson)
*****	Avoid the usage of Hick, prefer HCG
Details on Acronym: Hick
Hick	(Hickson)
*****	Avoid the usage of Hick, prefer HCG
Details on Acronym: HIDEEP
HIDEEP	(HI, Deep survey)
Write:	<<HIDEEP JHHMM+DDMM>> <<HIDEEP JHHMM+DDMMA>>
N:	173
Object:	HI (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	Extragalactic blind survey of 60deg(2) in Centaurus using the Parkes multibeam system.
Ref:	=2003MNRAS.346..787M
by	MINCHIN R.F. , DISNEY M.J., BOYCE P.J., DE BLOK W.J.G., PARKER Q.A., BANKS G.D., FREEMAN K.C., GARCIA D.A., GIBSON B.K., GROSSI M., HAYNES R.F., KNEZEK P.M., LANG R.H., MALIN D.F., PRICE R.M., STEWART I.M., WRIGHT A.E.
	Mon. Not. R. Astron. Soc., 346, 787-802 (2003)
	HIDEEP - an extragalactic blind survey for very low column-density neutral hydrogen.
o	Table 4: <HIDEEP JHHMM+DDMMA> N=173.
=E=	Catalogue in electronic form as J/MNRAS/346/787
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Hig
Hig	(Higgs)= (H) (Not yet in Simbad)
Write:	<<Hig NN>>
N:	31
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1966MNRAS.132...67H
by	HIGGS L.A.
	Mon. Not. R. Astron. Soc., 132, 67-78 (1966)
	The γ Cygni region of the Cygnus X radio source.
o	Table I: <Hig NN> (Nos 1-31)
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: HIGALBM
HIGALBM	(Herschel infrared Galactic Plane Survey Band-Merged)
Write:	<<HIGALBM GLLL.llll+BB.bbbb>> <<HIGALBM LLL.llll+BB.bbbb>> (not recognised by Simbad, but found in literature)
N:	62438+38484
Object:	Compact source (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	Hi-GAL (Herschel InfraRed Galactic Plane Survey) large-scale survey of the Galactic plane, performed with Herschel in five infrared continuum bands between 70 and 500 µm. The "high reliability" catalogue contains N=62438 sources, the "low reliability" catalogue contains N=38484 sources.
Ref:	=2017MNRAS.471..100E
by	ELIA D. , MOLINARI S., SCHISANO E., PESTALOZZI M., PEZZUTO S., MERELLO M., NORIEGA-CRESPO A., MOORE T.J.T., RUSSEIL D., MOTTRAM J.C., PALADINI R., STRAFELLA F., BENEDETTINI M., BERNARD J.P., DI GIORGIO A., EDEN D.J., FUKUI Y., PLUME R., BALLY J., MARTIN P.G., RAGAN S.E., JAFFA S.E., MOTTE F., OLMI L., SCHNEIDER N., TESTI L., WYROWSKI F., ZAVAGNO A., CALZOLETTI L., FAUSTINI F., NATOLI P., PALMEIRIM P., PIACENTINI F., PIAZZO L., PILBRATT G.L., POLYCHRONI D., BALDESCHI A., BELTRAN M.T., BILLOT N., CAMBRESY L., CESARONI R., GARCIA-LARIO P., HOARE M.G., HUANG M., JONCAS G., LIU S.J., MAIOLO B.M.T., MARSH K.A., MARUCCIA Y., MEGE P., PERETTO N., RYGL K.L.J., SCHILKE P., THOMPSON M.A., TRAFICANTE A., UMANA G., VENEZIANI M., WARD-THOMPSON D., WHITWORTH A.P., ARAB H., BANDIERAMONTE M., BECCIANI U., BRESCIA M., BUEMI C., BUFANO F., BUTORA R., CAVUOTI S., COSTA A., FIORELLINO E., HAJNAL A., HAYAKAWA T., KACSUK P., LETO P., LI CAUSI G., MARCHILI N., MARTINAVARRO-ARMENGOL S., MERCURIO A., MOLINARO M., RICCIO G., SANO H., SCIACCA E., TACHIHARA K., TORII K., TRIGILIO C., VITELLO F., YAMAMOTO H.
	Mon. Not. R. Astron. Soc., 471, 100-143 (2017)
	The Hi-GAL compact source catalogue - I. The physical properties of the clumps in the inner Galaxy (-71.0° < l < 67.0°).
o	<HIGALBM GLLL.llll+BB.bbbb> N=62438+38484.
=E=	Catalogue in electronic form as <J/MNRAS/471/100/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HIGALP
HIGALP	(Herschel infrared Galactic Plane Survey Preliminary catalogue)
Write:	<<HIGALP ALLL.llll+BB.llll>>
N:	123210+308509+280685+160972+85460
Object:	Compact source (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	The Herschel infrared Galactic Plane Survey (Hi-GAL) covers five wavebands at 70, 160, 250, 350 and 500µm. This first data release covers the inner Milky Way in the longitude range 68°≤l≤-70° in a \|b\|≥1° latitude strip. Hi-GAL DR1 catalogues contain N=123210+308509+280685+160972+85460 compact sources in the five bands. In format, the letter "A" stands for B (Blue: PACS 70µm), R (Red: PACS 160µm), "S" (PSW: SPIRE 250µm), M (PMW: SPIRE 350µm), L (PLW: SPIRE 500µm).
Ref:	=2016A&A...591A.149M
by	MOLINARI S. , SCHISANO E., ELIA D., PESTALOZZI M., TRAFICANTE A., PEZZUTO S., SWINYARD B.M., NORIEGA-CRESPO A., BALLY J., MOORE T.J.T., PLUME R., ZAVAGNO A., DI GIORGIO A.M., LIU S.J., PILBRATT G.L., MOTTRAM J.C., RUSSEIL D., PIAZZO L., VENEZIANI M., BENEDETTINI M., CALZOLETTI L., FAUSTINI F., NATOLI P., PIACENTINI F., MERELLO M., PALMESE A., DEL GRANDE R., POLYCHRONI D., RYGL K.L.J., POLENTA G., BARLOW M.J., BERNARD J.-P., MARTIN P.G., TESTI L., ALI B., ANDRE P., BELTRAN M.T., BILLOT N., CAREY S., CESARONI R., COMPIEGNE M., EDEN D., FUKUI Y., GARCIA-LARIO P., HOARE M.G., HUANG M., JONCAS G., LIM T.L., LORD S.D., MARTINAVARRO-ARMENGOL S., MOTTE F., PALADINI R., PARADIS D., PERETTO N., ROBITAILLE T., SCHILKE P., SCHNEIDER N., SCHULZ B., SIBTHORPE B., STRAFELLA F., THOMPSON M.A., UMANA G., WARD-THOMPSON D., WYROWSKI F.
	Astron. Astrophys., 591A, 149-149 (2016)
	Hi-GAL, the Herschel infrared Galactic Plane Survey: photometric maps and compact source catalogues. First data release for the inner Milky Way: +68°≥ l ≥70°.
o	<HIGALP ALLL.llll+BB.bbbb> N=123210+308509+280685+160972+85460.
=E=	Catalogue in electronic form as J/A+A/591/A149
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HII
HII	(HII)
*****	Avoid the usage of HII, prefer [W91]
Origin	of the Acronym: L (2006ApJ...648..355T)
Details on Acronym: HIJASS
HIJASS	(HI Jodrell All-Sky Survey)
*****	Avoid the usage of HIJASS, prefer [BMK2001b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HIJASS
HIJASS	(HI Jodrell All-Sky Survey)
Write:	<<HIJASS JHHMM+DDA>>
N:	222
Object:	HI G (SIMBAD class: Galaxy)
Stat.	in SIMBAD: 2003MNRAS.342..738L is completely incorporated.
Note:	First results from the HI Jodrell All-Sky Survey. Sample of N=222 galaxies.
Ref:	=2003MNRAS.342..738L
by	LANG R.H. , BOYCE P.J., KILBORN V.A., MINCHIN R.F., DISNEY M.J., JORDAN C.A., GROSSI M., GARCIA D.A., FREEMAN K.C., PHILLIPPS S., WRIGHT A.E.
	Mon. Not. R. Astron. Soc., 342, 738-758 (2003)
	First results from the HI Jodrell All Sky Survey: inclination-dependent selection effects in a 21-cm blind survey.
o	Table 2: The format is too short, a letter 'A' is added at the end of the format for different HIJASS galaxies with the same 'JHHMM+DD' format.
o	Table 2: <HIJASS JHHMM+DDA> N=222.
=E=	Catalogue in electronic form as J/MNRAS/342/738
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HIK2019]
[HIK2019]	(Hayashino+Inoue+Kousai+, 2019) (Not yet in Simbad)
Write:	<<[HIK2019] NNNNNN>>
N:	99
Object:	LBG (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	VLT VIMOS observations of N=99 Lyman Break Galaxies (LBGs) in the SSA22 field.
in source:	SSA 22
Ref:	=2019MNRAS.484.5868H
by	HAYASHINO T. , INOUE A.K., KOUSAI K., KASHIKAWA N., MAWATARI K., MATSUDA Y., TEJOS N., PROCHASKA J.X., IWATA I., NOLL S., BURGARELLA D., YAMADA T., AKIYAMA M.
	Mon. Not. R. Astron. Soc., 484, 5868-5887 (2019)
	Enhancement of H I absorption associated with the z = 3.1 large-scale proto-cluster and characteristic structures with AGNs sculptured over Gpc scale in the SSA22 field.
o	Table A1: <[HIK2019] NNNNNN> N=99 among (Nos 24239-151137).
=E=	Catalogue in electronic form as <J/MNRAS/484/5868/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Hilt
Hilt	(Hiltner)= Hiltner = (HN)
Write:	<<Hilt NNNN>>
N:	1259
Object:	OB* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1956ApJS....2..389H
by	HILTNER W.A.
	Astrophys. J., Suppl. Ser., 2, 389-462 (1956)
	Photometric, polarization, and spectroscopic observations of O and B stars.
o	misprint [GG53] 4 for [GG53] 14
o	Table 5: <Hilt NNNN> (Nos 1-1259)
=E=	Catalogue in electronic form as <J/ApJS/2/389/>
Details on Acronym: Hilt
Hilt	(Hiltner)
*****	Avoid the usage of Hilt, prefer [HJ56]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Hiltner
Hiltner	(Hiltner)
*****	Avoid the usage of Hiltner, prefer [H60]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Hiltner
Hiltner	(Hiltner)
====>	Equivalent to: Hilt
Details on Acronym: [HIM2022]
[HIM2022]	(Harikane+Inoue+Mawatari+, 2022)
Write:	<<[HIM2022] HDN>>
N:	3
Object:	Poss. LBG (SIMBAD class: Galaxy_Candidate = Galaxy Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=3 H-dropout Lyman break galaxy candidates at z∼12-16 in the COSMOS and SXDS fields. Use of UltraVISTA UKIDSS data.
in source:	NAME COSMOS Field
in source:	NAME SXDF
Ref:	=2022ApJ...929....1H
by	HARIKANE Y. , INOUE A.K., MAWATARI K., HASHIMOTO T., YAMANAKA S., FUDAMOTO Y., MATSUO H., TAMURA Y., DAYAL P., YUNG L.Y.A., HUTTER A., PACUCCI F., SUGAHARA Y., KOEKEMOER A.M.
	Astrophys. J., 929, 1-1 (2022)
	A Search for H-Dropout Lyman Break Galaxies at z ~ 12-16.
o	<[HIM2022] HDN> (Nos HD1-HD3).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [HIM85]
[HIM85]	(Heckman+Illingworth+Miley+, 1985)
Write:	<<[HIM85] 3C 218 A>>
N:	4
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=4 nearby galaxies to 3C 218.
Ref:	=1985ApJ...299...41H
by	HECKMAN T.M. , ILLINGWORTH G.D., MILEY G.K., VAN BREUGEL W.J.M.
	Astrophys. J., 299, 41-58 (1985)
	The kinematics of stars and gas in radio galaxies.
o	App.B, Table 8: <[HIM85] 3C 218 A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HIO2012]
[HIO2012]	(Hayashi+Itoh+Oasa, 2012)
Write:	<<[HIO2012] BRC NN NNN>>
N:	2099
Object:	Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Note:	UKIRT WFCam NIR observations of N=2099 YSO candidates in 32 bright-rimmed clouds (BRCs, see SFO).
Ref:	=2012PASJ...64...96H
by	HAYASHI Y. , ITOH Y., OASA Y.
	PASJ, 64, 96 (2012)
	Near-infrared survey of bright rimmed clouds.
o	Table 2: <[HIO2012] BRC NN NNN> N=2099.
=E=	Catalogue in electronic form as J/PASJ/64/96
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HIP
HIP	(Hipparcos catalogue)
Write:	<<HIP NNNNNNA>> <<HIP NNN NNNA>> (not recognised by Simbad, but found in literature)
N:	118218+117955+24588
Object:	* (SIMBAD class: Star)
Note:	Results of Hipparcos mission.
Ref:	=1997HIP...C......0E
by	ESA
	European Space Agency SP-1200, 0-None (1997)
	The Hipparcos and Tycho Catalogues (vol. 1-17).
o	See 1997A&A...323L..49P and 1998A&A...335L..65H for more details.
o	<HIP NNNNNN> N=118218. <TYC FFFF NNNNN N> N=1058332.
Ref:	=2007A&A...474..653V
by	VAN LEEUWEN F.
	Astron. Astrophys., 474, 653-664 (2007)
	Validation of the new Hipparcos reduction.
o	Catalog: <HIP NNNNNN> N=117955 among (Nos 1-120404).
Ref:	=1997A&A...323L..49P
by	PERRYMAN M.A.C. , LINDEGREN L., KOVALEVSKY J., HOG E., BASTIAN U., BERNACCA P.L., CREZE M., DONATI F., GRENON M., GREWING M., VAN LEEUWEN F., VAN DER MAREL H., MIGNARD F., MURRAY C.A., LE POOLE R.S., SCHRIJVER H., TURON C., ARENOU F., FROESCHLE M., PETERSEN C.S.
	Astron. Astrophys., 323, 49-52 (1997)
	The Hipparcos Catalogue.
o	reprint in the special issue (500/1) : 2009A&A...500..501P
o	<HIP NNNNNN> N=118218 among (Nos 1-120416).
=E=	Catalogue in electronic form as I/239
=E=	Catalogue in electronic form as I/259
=E=	Catalogue in electronic form as I/311
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HIP
HIP	(Hipparcos catalogue)
Write:	<<HIP NNNNNNAa>> <<HIP NNN NNNAa>> (not recognised by Simbad, but found in literature)
Object:	Planet (SIMBAD class: Planet = Extra-solar Planet)
Note:	Suffix a added to the original format, to follow in SIMBAD the usage found in the literature regarding planets around stars or multiple star systems in the Hipparcos Catalogue.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HIP2003]
[HIP2003]	(Helmi+Ivezic+Prada+, 2003)
Write:	<<[HIP2003] JHHMMSS.s+DDMMSS.s>>
N:	29
Object:	Poss. Giant (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Sloan Digital Sky Survey (SDSS) data are used for a photometric selection of metal-poor halo giants.
Ref:	=2003ApJ...586..195H
by	HELMI A. , IVEZIC Z., PRADA F., PENTERICCI L., ROCKOSI C.M., SCHNEIDER D.P., GREBEL E.K., HARBECK D., LUPTON R.H., GUNN J.E., KNAPP G.R., STRAUSS M.A., BRINKMANN J.
	Astrophys. J., 586, 195-200 (2003)
	Selection of metal-poor giant stars using the Sloan Digital Sky Survey photometric system.
o	Table 1: <[HIP2003] JHHMMSS.s+DDMMSS.s> N=29.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HIPASS
HIPASS	(HI Parkes All Sky Survey)
Write:	<<HIPASS JHHMM+DDa>>
N:	4315+5317
Object:	HI G (SIMBAD class: HI = HI (21cm) Source)
Note:	HI Parkes All Sky Survey. 2006MNRAS.371.1855W: northern extension of the HIPASS catalogue (NHICAT). See also [K99b], [KSM2000].
Ref:	=2002AJ....124..690K
by	KILBORN V.A. , WEBSTER R.L., STAVELEY-SMITH L., MARQUARDING M., BANKS G.D., BARNES D.G., BHATHAL R., DE BLOK W.J.G., BOYCE P.J., DISNEY M.J., DRINKWATER M.J., EKERS R.D., FREEMAN K.C., GIBSON B.K., HENNING P.A., HOWLETT M., JERJEN H., KNEZEK P.M., KORIBALSKI B., MALIN D.F., MINCHIN R.F., MOULD J.R., O'BRIEN J.C., OOSTERLOO T., ORTIZ P.F., PRICE R.M., PUTMAN M.E., RYDER S.D., SADLER E.M., STEWART I.M., STOOTMAN F., WONG O.I., WRIGHT A.E.
	Astron. J., 124, 690-705 (2002)
	A catalog of H I-selected galaxies from the south celestial cap region of sky.
o	Table 1: <HIPASS JHHMM+DD> N=536.
Ref:	=2003MNRAS.343.1195R
by	RYAN-WEBER E.V. , WEBSTER R.L., STAVELEY-SMITH L.
	Mon. Not. R. Astron. Soc., 343, 1195-1206 (2003)
	The column density distribution function at z = 0 from HI selected galaxies.
o	(Erratum) erratum vol. 356, p. 1600 (2005)
o	Table A1: <HIPASS JHHMM+DD> N=35.
Ref:	=2004MNRAS.350.1195M
by	MEYER M.J. , ZWAAN M.A., WEBSTER R.L., STAVELEY-SMITH L., RYAN-WEBER E., DRINKWATER M.J., BARNES D.G., HOWLETT M., KILBORN V.A., STEVENS J., WAUGH M., PIERCE M.J., BHATHAL R., DE BLOK W.J.G., DISNEY M.J., EKERS R.D., FREEMAN K.C., GARCIA D.A., GIBSON B.K., HARNETT J., HENNING P.A., JERJEN H., KESTEVEN M.J., KNEZEK P.M., KORIBALSKI B.S., MADER S., MARQUARDING M., MINCHIN R.F., O'BRIEN J., OOSTERLOO T., PRICE R.M., PUTMAN M.E., RYDER S.D., SADLER E.M., STEWART I.M., STOOTMAN F., WRIGHT A.E.
	Mon. Not. R. Astron. Soc., 350, 1195-1209 (2004)
	The HIPASS catalogue - I. Data presentation.
o	Table 6: <HIPASS JHHMM+DDa> N=4315.
Ref:	=2006MNRAS.371.1855W
by	WONG O.I. , RYAN-WEBER E.V., GARCIA-APPADOO D.A., WEBSTER R.L., STAVELEY-SMITH L., ZWAAN M.A., MEYER M.J., BARNES D.G., KILBORN V.A., BHATHAL R., DE BLOK W.J.G., DISNEY M.J., DOYLE M.T., DRINKWATER M.J., EKERS R.D., FREEMAN K.C., GIBSON B.K., GUROVICH S., HARNETT J., HENNING P.A., JERJEN H., KESTEVEN M.J., KNEZEK P.M., KORIBALSKI B.S., MADER S., MARQUARDING M., MINCHIN R.F., O'BRIEN J., PUTMAN M.E., RYDER S.D., SADLER E.M., STEVENS J., STEWART I.M., STOOTMAN F., WAUGH M.
	Mon. Not. R. Astron. Soc., 371, 1855-1864 (2006)
	The Northern HIPASS catalogue - data presentation, completeness and reliability measures.
o	Table 5: <HIPASS JHHMM+DDa> N=5317.
=E=	Catalogue in electronic form as J/AJ/124/690
=E=	Catalogue in electronic form as VIII/73
=E=	Catalogue in electronic form as <VIII/89/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HIPASS
HIPASS	(HI Parkes All Sky Survey)
*****	Avoid the usage of HIPASS, prefer [K99b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HIPASS
HIPASS	(HI Parkes All Sky Survey)
*****	Avoid the usage of HIPASS, prefer [KSM2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HIPASS
HIPASS	(HI Parkes All Sky Survey)
*****	Avoid the usage of HIPASS, prefer [PDS2002]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HIPASS
HIPASS	(HI Parkes All Sky Survey)
*****	Avoid the usage of HIPASS, prefer [RKS2002]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HIPASS
HIPASS	(HI Parkes All Sky Survey)
*****	Avoid the usage of HIPASS, prefer [WDW2002]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HIPEQ
HIPEQ	(HI Parkes Equatorial Survey)
Write:	<<HIPEQ JHHMM+DDa>> <<HIPEQ HHMM+DDa>> (not recognised by Simbad, but found in literature)
N:	195
Object:	G (SIMBAD class: Galaxy)
Note:	Parkes 64-m radio telescope HI observations of galaxies. Use of SDSS DR2 data.
Ref:	=2009MNRAS.394..340G
by	GARCIA-APPADOO D.A. , WEST A.A., DALCANTON J.J., CORTESE L., DISNEY M.J.
	Mon. Not. R. Astron. Soc., 394, 340-356 (2009)
	Correlations among the properties of galaxies found in a blind HI survey, which also have SDSS optical data.
o	Table 2: <HIPEQ JHHMM+DDa> N=195.
=E=	Catalogue in electronic form as J/MNRAS/394/340
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HIPPIES
HIPPIES	(Hubble Infrared Pure Parallel Imaging Extragalactic Survey)
Write:	<<HIPPIES YsDropNN>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFC3 observations as part of the Hubble Infrared Pure Parallel Imaging Extragalactic Survey (HIPPIES). N=3 Y-dropout sources. See http://archive.stsci.edu/prepds/hippies/
Ref:	=2011ApJ...728L..22Y
by	YAN H. , YAN L., ZAMOJSKI M.A., WINDHORST R.A., McCARTHY P.J., FAN X., ROTTGERING H.J.A., KOEKEMOER A.M., ROBERTSON B.E., DAVE R., CAI Z.
	Astrophys. J., 728L, 22 (2011)
	Probing very bright end of galaxy luminosity function at z ≳ 7 using Hubble space telescope pure parallel observations.
o	Table 1: <HIPPIES YsDropNN> (Nos 01-03).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HIR
HIR	(HIPASS Reprocessed) (Not yet in Simbad)
Write:	<<HIR JHHMM+DDMM>> <<HIR HHMM+DDMM>> (not recognised by Simbad, but found in literature)
N:	203
Object:	HI (SIMBAD class: HI = HI (21cm) Source)
Note:	N=203 objects found in HIPASS reprocessed data of the region observed for the Westerbork Virgo Filament Survey (WVFS).
in source:	NAME Virgo Cluster
Ref:	=2011A&A...533A.122P
by	POPPING A. , BRAUN R.
	Astron. Astrophys., 533A, 122-122 (2011)
	Diffuse neutral hydrogen in the H I Parkes All Sky Survey.
o	Table 1: <HIR JHHMM+DDMM> N=203.
=E=	Catalogue in electronic form as J/A+A/533/A122
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Hirahara
Hirahara	(Hirahara+)
*****	Avoid the usage of Hirahara, prefer TMC
Details on Acronym: HIROCS
HIROCS	(Heidelberg IR-Optical Cluster Survey)
Write:	<<HIROCS JHHMMSS.s+DDMMSS>>
N:	15
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Heidelberg IR-Optical Cluster Survey in the COSMOS field. See also ([ZRW2007]).
in source:	NAME COSMOS Field
Ref:	=2007A&A...474L...5Z
by	ZATLOUKAL M. , ROESER H.-J., WOLF C., HIPPELEIN H., FALTER S.
	Astron. Astrophys., 474L, 5-8 (2007)
	Distant galaxy clusters in the COSMOS field found by HIROCS.
o	Table 2, col(1): <[ZRW2007] NN> (Nos 1-15) = Table 2, col(2): <HIROCS JHHMMSS.s+DDMMSS> N=15.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HIS2023]
[HIS2023]	(Hyun+Im+Smail+Cotton+, 2023) (Not yet in Simbad)
Write:	<<[HIS2023] NNN>>
N:	756
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA 3GHz observations of N=756 radio sources in the James Webb Space Telescope Time-Domain field (JWST-TDF). See also S2TDF.
Ref:	=2023ApJS..264...19H
by	HYUN M. , IM M., SMAIL I.R., COTTON W.D., BIRKIN J.E., KIKUTA S., SHIM H., WILLMER C.N.A., CONDON J.J., WINDHORST R.A., COHEN S.H., JANSEN R.A., LY C., MATSUDA Y., FAZIO G.G., SWINBANK A.M., YAN H.
	Astrophys. J., Suppl. Ser., 264, 19 (2023)
	The JCMT SCUBA-2 Survey of the James Webb Space Telescope North Ecliptic Pole Time-Domain Field.
o	Table 3: <[HIS2023] NNN> (Nos 1-756). Table 4: <S2TDF JHHMMSS+DDMMSS> N=114 = <S2TDF.NNNN> (Nos 0001-0114), <S2TDF.NNNN.N> N=133 among (Nos 0001.0-0114.0).
=E=	Catalogue in electronic form as <J/ApJS/264/19/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: HiTS
HiTS	(High Cadence Transient Survey)
Write:	<<HiTS JHHMMSS+DDMMSS>> <<HiTS HHMMSS+DDMMSS>> (not recognised by Simbad, but found in literature)
N:	3+173+3485
Object:	Transient + V* + QSO (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	The High cadence Transient Survey (HiTS) aims at discovering and study transients objects, using data taken with the Dark Energy Camera (DECam) at the CTIO Blanco 4m telescope. The first data release is described in 2018AJ....156..186M and can be accessed in the project archive http://astro.cmm.uchile.cl/HiTS/
Ref:	=2017ApJ...845L..10M
by	MEDINA G.E. , MUNOZ R.R., VIVAS A.K., FORSTER F., CARLIN J.L., MARTINEZ J., GALBANY L., GONZALEZ-GAITAN S., HAMUY M., DE JAEGER T., MAUREIRA J.C., MARTIN J.S.
	Astrophys. J., 845L, 10-10 (2017)
	Serendipitous discovery of RR Lyrae stars in the Leo V ultra-faint galaxy.
o	<HiTS JHHMMSS+DDMMSS> N=3.
Ref:	=2018ApJ...855...43M
by	MEDINA G.E. , MUNOZ R.R., VIVAS A.K., CARLIN J.L., FORSTER F., MARTINEZ J., GALBANY L., GONZALEZ-GAITAN S., HAMUY M., DE JAEGER T., MAUREIRA J.C., MARTIN J.S.
	Astrophys. J., 855, 43-43 (2018)
	Discovery of distant RR Lyrae stars in the Milky Way using DECam.
o	Tables 1+5+6: <HiTS JHHMMSS+DDMMSS> N=173.
Ref:	=2018AJ....156..186M
by	MARTINEZ-PALOMERA J. , FORSTER F., PROTOPAPAS P., MAUREIRA J.C., LIRA P., CABRERA-VIVES G., HUIJSE P., GALBANY L., DE JAEGER T., GONZALEZ-GAITAN S., MEDINA G., PIGNATA G., MARTIN J.S., HAMUY M., MUNOZ R.R.
	Astron. J., 156, 186-186 (2018)
	The High Cadence Transit Survey (HiTS): compilation and characterization of light-curve catalogs.
o	<HiTS JHHMMSS+DDMMSS> N=3485.
=E=	Catalogue in electronic form as <J/ApJ/855/43/>
=E=	Catalogue in electronic form as <J/AJ/156/186/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HiZELS
HiZELS	(High-redshift(Z) Emission Line Survey)
Write:	<<HiZELS -{COSMOS\|UDS}-{NB921\|NBJ\|NBH\|NBK}-{S12}-NNNNNN>> <<HiZELS -COSMOS-NBK-S12B-NNNNNN>> <<HiZELS -{COSMOS\|UDS}-{NB921\|NBJ\|NBH\|NBK}-{DTC}-{S12}-NNNNNN>> (not recognised by Simbad, but found in literature)
N:	9776+1251+1141+1758
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	Subaru (NB921), UKIRT (NB_J, NB_H, NB_K), ESO VLT HAWK-I observations of Hα star-forming galaxies in the COSMOS and UDS fields, as part of the High-redshift(Z) Emission Line Survey (HiZELS).
Ref:	=2013MNRAS.428.1128S
by	SOBRAL D. , SMAIL I., BEST P.N., GEACH J.E., MATSUDA Y., STOTT J.P., CIRASUOLO M., KURK J.
	Mon. Not. R. Astron. Soc., 428, 1128-1146 (2013)
	A large Hα survey at z = 2.23, 1.47, 0.84 and 0.40: the 11 Gyr evolution of star-forming galaxies from HiZELS.
o	Tables a1-a4: <HiZELS-COSMOS-NB921-S12-NNNNNN>, <HiZELS-COSMOS-NBJ-S12-NNNNNN>, <HiZELS-COSMOS-NBH-S12-NNNNNN>, <HiZELS-COSMOS-NBK-S12-NNNNNN>, <HiZELS-UDS-NB921-S12-NNNNNN>, <HiZELS-UDS-NBJ-S12-NNNNNN>, <HiZELS-UDS-NBH-S12-NNNNNN>, <HiZELS-UDS-NBK-S12-NNNNNN>, <HiZELS-COSMOS-NBK-S12B-NNNNNN>, N=9776+1251+1141+1758.
=E=	Catalogue in electronic form as <J/MNRAS/428/1128/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HIZOA
HIZOA	(HI, Zone Of Avoidance)
Write:	<<HIZOA JHHMM+DDA>>
N:	42+77+882+729+340
Object:	G (SIMBAD class: Galaxy)
Note:	Hydrogen survey for galaxies in several regions. See also HIZSS.
Ref:	=2000AJ....119.1627J
by	JURASZEK S.J. , STAVELEY-SMITH L., KRAAN-KORTEWEG R.C., GREEN A.J., EKERS R.D., HAYNES R.F., HENNING P.A., KESTEVEN M.J., KORIBALSKI B., PRICE R.M., SADLER E.M., SCHROEDER A.
	Astron. J., 119, 1627-1637 (2000)
	A blind H I survey for galaxies in the zone of avoidance, 308°≤l≤332°.
o	Table 1: <HIZOA JHHMM+DD> N=42.
Ref:	=2005AJ....129..220D
by	DONLEY J.L. , STAVELEY-SMITH L., KRAAN-KORTEWEG R.C., ISLAS-ISLAS J.M., SCHROEDER A., HENNING P.A., KORIBALSKI B., MADER S., STEWART I.
	Astron. J., 129, 220-238 (2005)
	The H I Parkes zone of avoidance survey: the northern extension.
o	Table 1: <HIZOA JHHMM+DDA> N=77.
Ref:	=2016AJ....151...52S
by	STAVELEY-SMITH L. , KRAAN-KORTEWEG R.C., SCHRODER A.C., HENNING P.A., KORIBALSKI B.S., STEWART I.M., HEALD G.
	Astron. J., 151, 52 (2016)
	The Parkes H I zone of avoidance survey.
Ref:	=2016MNRAS.457.2366S
by	SAID K. , KRAAN-KORTEWEG R.C., STAVELEY-SMITH L., WILLIAMS W.L., JARRETT T.H., SPRINGOB C.M.
	Mon. Not. R. Astron. Soc., 457, 2366-2376 (2016)
	NIR Tully-Fisher in the Zone of Avoidance - II. 21 cm H I-line spectra of southern ZOA galaxies.
o	Tables 2-3: <HIZOA JHHMM+DDA> N=103+237.
Ref:	=2016MNRAS.462.3386S
by	SAID K. , KRAAN-KORTEWEG R.C., JARRETT T.H., STAVELEY-SMITH L., WILLIAMS W.L.
	Mon. Not. R. Astron. Soc., 462, 3386-3400 (2016)
	NIR Tully-Fisher in the Zone of Avoidance - III. Deep NIR catalogue of the HIZOA galaxies.
o	Tables 2a-2b, col(1): <ZOA JHHMMSS.sss+DDMMSS.ss> N=129+914. Tables 2a-2b: <HIZOA JHHMM+DDA> N=52+677.
=E=	Catalogue in electronic form as J/AJ/129/220
=E=	Catalogue in electronic form as <J/MNRAS/462/3386/>
=E=	Catalogue in electronic form as <J/AJ/151/52/>
=E=	Catalogue in electronic form as <J/MNRAS/457/2366/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HIZSS
HIZSS	(HI, Zone of avoidance, Southern Survey)
Write:	<<HIZSS NNN>>
N:	110
Object:	HI G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Survey of HI bright galaxies in the southern zone of avoidance. See also HIZOA
Ref:	=2000AJ....119.2686H
by	HENNING P.A. , STAVELEY-SMITH L., EKERS R.D., GREEN A.J., HAYNES R.F., JURASZEK S., KESTEVEN M.J., KORIBALSKI B., KRAAN-KORTEWEG R.C., PRICE R.M., SADLER E.M., SCHROEDER A.
	Astron. J., 119, 2686-2698 (2000)
	H I-bright galaxies in the southern zone of avoidance.
o	Table 2: <HIZSS NNN> (Nos 1-110).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HJ
HJ	(Herschel J.)
*****	Avoid the usage of HJ, prefer Her
Details on Acronym: HJ
HJ	(Herbig+Jones)
*****	Avoid the usage of HJ, prefer [HJ83]
Origin	of the Acronym: L (1997A&A...324..690P)
Details on Acronym: [HJ56]
[HJ56]	(Hiltner+Johnson, 1956)= (Hilt)
Write:	<<[HJ56] NNN>>
N:	262
Object:	O * (SIMBAD class: Star)
Ref:	=1956ApJ...124..367H
by	HILTNER W.A. , JOHNSON H.L.
	Astrophys. J., 124, 367-378 (1956)
	The law of interstellar reddening and absorption.
o	<[HJ56] NNN> (Nos 1-262)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJ83]
[HJ83]	(Herbig+Jones, 1983)= (HJ)
Write:	<<[HJ83] NNN>>
N:	63 among 133
Object:	* (SIMBAD class: Star)
Note:	Table III: N = 63 stars among (Nos 1-133), near NGC 1333
in source:	NGC 1333
Ref:	=1983AJ.....88.1040H
by	HERBIG G.H. , JONES B.F.
	Astron. J., 88, 1040-1052 (1983)
	Proper motions of Herbig-Haro objects. III. HH-7 through -11, HH-12, and HH-32.
o	<HH NNA> Nos 7, 10, 11, 12, 17. Table III: <[HJ83] NNN> N=63 among 111
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJ91]
[HJ91]	(Hyland+Jones, 1991)
Write:	<<[HJ91] PN>>
N:	4
Object:	Poss. Protostar (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
in source:	Magellanic Clouds:LMC:30 Dor Nebula = 30 Dor Nebula
Ref:	=1991IAUS..148..202H
by	HYLAND A.R. , JONES T.J.
	148th Symposium of the IAU, held in Sydney, Australia, July 9-13, 1990. Ed. R. Haynes and D. Milne. "The Magellanic Clouds", 148, 202-204 (1991)
	Candidate protostars in the vicinity of 30 Doradus.
o	Table 1: <[HJ91] PN> (Nos P1-P4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJ96]
[HJ96]	(Henriksen+Jones, 1996)
Write:	<<[HJ96] ANNNNW>>
N:	4
Object:	Subcluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	ROSAT PSPC observations of subclusters in bimodal systems A3395 and A3528.
in source:	ACO 3395
in source:	ACO 3528
Ref:	=1996ApJ...465..666H
by	HENRIKSEN M. , JONES C.
	Astrophys. J., 465, 666-679 (1996)
	An X-ray and optical study of clusters in formation.
o	Table 1: <[HJ96] ANNNNW> (Nos A3395N, A3395S, A3528N, A3528S).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJA2010]
[HJA2010]	(Harvey+Jaffe+Allers+, 2010)
Write:	<<[HJA2010] JHHMMSS.ss+DDMMSS.s>>
N:	18
Object:	Poss. Brown Dwarf (SIMBAD class: BrownD*_Candidate = Brown Dwarf Candidate)
Stat:	is completely incorporated in Simbad
Note:	CTIO Blanco 4m telescope NIR and optical imaging and Spitzer IRAC observations of N=18 very low-mass brown dwarf candidates in Ophiuchus.
in source:	NAME Ophiuchus Cloud
Ref:	=2010ApJ...720.1374H
by	HARVEY P.M. , JAFFE D.T., ALLERS K., LIU M.
	Astrophys. J., 720, 1374-1379 (2010)
	A Spitzer search for planetary-mass brown dwarfs with circumstellar disks: candidate selection.
o	Table 2: <[HJA2010] JHHMMSS.ss+DDMMSS.s> N=18.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJB2000]
[HJB2000]	(Haynes+Jore+Barrett+, 2000)
Write:	<<[HJB2000] HHMMSS.s+DDMMSS>>
N:	1+1+4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio-sources detected in the field of NGC 3626 (N=1), NGC 3900 (N=1), and NGC 4772 (N=4).
Ref:	=2000AJ....120..703H
by	HAYNES M.P. , JORE K.P., BARRETT E.A., BROEILS A.H., MURRAY B.M.
	Astron. J., 120, 703-727 (2000)
	Kinematic evidence of minor mergers in normal Sa galaxies: NGC 3626, NGC 3900, NGC 4772, and NGC 5854.
o	p.708-709: <[HJB2000] HHMMSS.s+DDMMSS> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJB2016]
[HJB2016]	(Heywood+Jarvis+Baker+, 2016)
Write:	<<[HJB2016] JHHMMSS.s+DDMMSSA>>
N:	5628+6062+56+32
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Jansky VLA 1-2GHz observations of N=5674+6094 point and Gaussian components in SDSS Stripe 82.
Ref:	=2016MNRAS.460.4433H
by	HEYWOOD I. , JARVIS M.J., BAKER A.J., BANNISTER K.W., CARVALHO C.S., HARDCASTLE M., HILTON M., MOODLEY K., SMIRNOV O.M., SMITH D.J.B., WHITE S.V., WOLLACK E.J.
	Mon. Not. R. Astron. Soc., 460, 4433-4452 (2016)
	A deep/wide 1-2 GHz snapshot survey of SDSS Stripe 82 using the Karl G. Jansky Very Large Array in a compact hybrid configuration.
o	Table 1: <[HJB2016] JHHMMSS.s+DDMMSS> N=5628+6062, <[HJB2016] JHHMMSS.s+DDMMSSA> N=46+32.
=E=	Catalogue in electronic form as <J/MNRAS/460/4433/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJB85]
[HJB85]	(Ho+Jackson+Barrett+, 1985)
Write:	<<[HJB85] Sgr A-A>> <<[HJB85] Sgr A-ANN>> <<[HJB85] Sgr A-ANNa>>
N:	15+22+10
Object:	(Rad) + (IR) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio in Sgr A, (Nos A-O) and components 'ANN'. Some objects are coming from the PhD Thesis of Yusef-Zadeh in 1986, and are found later in the literature. See also EVSG, [CSE99].
in source:	NAME Sgr A
Ref:	=1985ApJ...288..575H
by	HO P.T.P. , JACKSON J.M., BARRETT A.H., ARMSTRONG J.T.
	Astrophys. J., 288, 575-579 (1985)
	Interactions between the continuum sources in the Galactic Center and their immediate molecular environment.
o	Table 1: <[HJB85] Sgr A-A> (Nos Sgr A-A to Sgr A-G)
Ref:	=1987ApJ...320..545Y
by	YUSEF-ZADEH F. , MORRIS M.
	Astrophys. J., 320, 545-561 (1987)
	Structural details of the Sagittarius A complex: evidence for a large-scale poloidal magnetic field in the Galactic Center region.
o	Table 1: <[HJB85] Sgr A-A> (Nos H-M) added, <[HJB85] Sgr A-AN> (Nos C1-C2, H1-H8, I1-I3, L1-L3).
Ref:	=2001AJ....121.2681L
by	LANG C.C. , GOSS W.M., MORRIS M.
	Astron. J., 121, 2681-2705 (2001)
	A VLA H92α recombination line study of the arched filament H II complex near the Galactic Center.
o	Table 4: <[LGM2001] A> (Nos A-N). Table 5: <[HJB85] Sgr A-HNN> (Nos H9-H13) added.
Ref:	=2019ApJ...877...22H
by	HANKINS M.J. , LAU R.M., MILLS E.A.C., MORRIS M.R., HERTER T.L.
	Astrophys. J., 877, 22-22 (2019)
	SOFIA/FORCAST observations of the Sgr A-H H II regions: using dust emission to elucidate the heating sources.
o	Tables 2/5: <[HJB85] Sgr A-HNN> (Nos H14-H21) added. Table 5: <[HJB85] Sgr A-HNNa> (Nos H22c, H23c) added. Table 4: <[HLM2019] Sgr A-HNWW> (Nos H2NE, H2SW, H3S, H5E and H5W) N=5, <[HLM2019] Sgr A-H3NN> (Nos H3N1, H3N2) N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJC2005]
[HJC2005]	(Hasegan+Jordan+Cote+, 2005)
Write:	<<[HJC2005] NNNN-N>>
N:	18
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Search for DGTOs (Dwarf Globular Transition Objects) in the VCC Virgo Cluster Survey. The first digits 'NNNN' in the format stands for the VCC NNNN galaxy.
in source:	NAME Virgo Cluster
Ref:	=2005ApJ...627..203H
by	HASEGAN M. , JORDAN A., COTE P., DJORGOVSKI S.G., McLAUGHLIN D.E., BLAKESLEE J.P., MEI S., WEST M.J., PENG E.W., FERRARESE L., MILOSAVLJEVIC M., TONRY J.L., MERRITT D.
	Astrophys. J., 627, 203-223 (2005)
	The ACS Virgo cluster survey. VII. Resolving the connection between globular clusters and ultracompact dwarf galaxies.
o	Table 9: <[HJC2005] NNNN-N> N=18.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJC2008]
[HJC2008]	(Hogan+Jameson+Casewell+, 2008) (Not yet in Simbad)
Write:	<<[HJC2008] NN>>
N:	12
Object:	* (SIMBAD class: Star)
Note:	N=12 brown dwarfs in the Hyades open cluster. Use of archival 2MASS and UKIDSS surveys.
in source:	Hyades = Cl Melotte 25
Ref:	=2008MNRAS.388..495H
by	HOGAN E. , JAMESON R.F., CASEWELL S.L., OSBOURNE S.L., HAMBLY N.C.
	Mon. Not. R. Astron. Soc., 388, 495-499 (2008)
	L dwarfs in the Hyades.
o	Table 1: <[HJC2008] NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJD93]
[HJD93]	((Benedict)+Higdon+Jefferys+Duncombe+, 1993)
*****	Avoid the usage of [HJD93], prefer [BHJ93]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJF2013]
[HJF2013]	(Hoq+Jackson+Foster+, 2013)
Write:	<<[HJF2013] GLLL.lll+BB.bbb>>
N:	333
Object:	Clump (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	Mopra Telescope molecular line observations of N=333 star-forming clumps with the Millimetre Astronomy Legacy Team 90 GHz MALT90 survey. Target sources were chosen from the APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) survey.
Ref:	=2013ApJ...777..157H
by	HOQ S. , JACKSON J.M., FOSTER J.B., SANHUEZA P., GUZMAN A., WHITAKER J.S., CLAYSMITH C., RATHBORNE J.M., VASYUNINA T., VASYUNIN A.
	Astrophys. J., 777, 157 (2013)
	Chemical evolution in high-mass star-forming regions: results from the MALT90 survey.
o	Tables 1, 5: <[HJF2013] GLLL.lll+BB.bbb> N=333.
=E=	Catalogue in electronic form as J/ApJ/777/157
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJH2006]
[HJH2006]	(Haikala+Juvela+Harju+, 2006)
Write:	<<[HJH2006] CG 12-W>> <<[HJH2006] CG 12-WW>>
N:	3
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	APEX telescope C18O observations of cores in the globule CG 12.
in source:	CG 12
Ref:	=2006A&A...454L..71H
by	HAIKALA L.K. , JUVELA M., HARJU J., LEHTINEN K., MATTILA K., DUMKE M.
	Astron. Astrophys., 454, 71-74 (2006)
	C^{18}O (3-2) observations of the Cometary Globule CG 12: a cold core and a C^{18}O hot spot.
o	Paragr. 3.1: <[HJH2006] CG 12-W> (Nos CG 12-N, CG 12-S).
Ref:	=2007A&A...466..191H
by	HAIKALA L.K. , OLBERG M.
	Astron. Astrophys., 466, 191-200 (2007)
	The structure of the cometary globule CG 12: a high-latitude star-forming region.
o	Fig.1: <[HJH2006] CG 12-WW> (No. CG 12-SW) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJH2016]
[HJH2016]	(Hindson+Johnston-Hollitt+Hurley-Walker+, 2016)
Write:	<<[HJH2016] GLLL.ll+BB.bb>>
N:	302
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Murchison Widefield Array (MWA) observations (between 72 and 231MHz) of N=302 HII regions between 260°<l<340°, as part of the GLEAM survey.
Ref:	=2016PASA...33...20H
by	HINDSON L. , JOHNSTON-HOLLITT M., HURLEY-WALKER N., CALLINGHAM J.R., SU H., MORGAN J., BELL M., BERNARDI G., BOWMAN J.D., BRIGGS F., CAPPALLO R.J., DESHPANDE A.A., DWARAKANATH K.S., FOR B.-Q., GAENSLER B.M., GREENHILL L.J., HANCOCK P., HAZELTON B.J., KAPIN A.D., KAPLAN D.L., LENC E., LONSDALE C.J., MCKINLEY B., MCWHIRTER S.R., MITCHELL D.A., MORALES M.F., MORGAN E., OBEROI D., OFFRINGA A., ORD S.M., PROCOPIO P., PRABU T., UDAYA SHANKAR N., SRIVANI K.S., STAVELEY-SMITH L., SUBRAHMANYAN R., TINGAY S.J., WAYTH R.B., WEBSTER R.L., WILLIAMS A., WILLIAMS C.L., WU C., ZHENG Q.
	PASA, 33, 20-20 (2016)
	A Large Scale, Low Frequency Murchison Widefield Array Survey of Galactic HII regions between 260 < l < 340.
o	Table 2: <[HJH2016] GLLL.ll+BB.bb> N=302.
=E=	Catalogue in electronic form as <J/other/PASA/33.20/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJK2000]
[HJK2000]	(Hurt+Jarrett+Kirkpatrick+, 2000)= (GC) = (2MASS)
Write:	<<[HJK2000] GCNN>>
N:	2
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Note:	2MASS discoveries: N=2 globular clusters.
Ref:	=2000AJ....120.1876H
by	HURT R.L. , JARRETT T.H., KIRKPATRICK J.D., CUTRI R.M., SCHNEIDER S.E., SKRUTSKIE M., VAN DRIEL W.
	Astron. J., 120, 1876-1883 (2000)
	Serendipitous 2MASS discoveries near the galactic plane: a spiral galaxy and two globular clusters.
o	Tables 1, 3: <[HJK2000] GCNN> (Nos GC01-GC02). Fig.1: <2MASXI JHHMMSSs+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HJM
HJM	(Hyland+Jones+Mitchell)= (C) = (Cha) = (Cham)
Write:	<<HJM AFF-NNa>>
N:	121
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	In the format 'AFF' stands for (C1 to C10) or (E1 to E4) 'blocks'. Numbering of objects in the 'block' C1 is continued in the second ref.
in source:	NAME Cha Dark Cloud
Ref:	=1982MNRAS.201.1095H
by	HYLAND A.R. , JONES T.J., MITCHELL R.M.
	Mon. Not. R. Astron. Soc., 201, 1095-1117 (1982)
	A study of the Chamaeleon dark cloud complex: survey, structure and embedded sources.
o	<HJM AFF-NN> N=109.
Ref:	=1985AJ.....90.1191J
by	JONES T.J. , HYLAND A.R., HARVEY P.M., WILKING B.A., JOY M.
	Astron. J., 90, 1191-1195 (1985)
	The Chamaeleon dark cloud complex. II. A deep survey around HD 97300.
o	<HJM AF-NN> continuation, block C1
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HJM2004]
[HJM2004]	(Harrison+Johnson+McArthur+, 2004)
Write:	<<[HJM2004] WZ Sge Ref N>> <<[HJM2004] YZ Cnc Ref N>> <<[HJM2004] RU Peg Ref N>>
N:	5+4+5
Object:	* (SIMBAD class: Star)
Note:	Reference stars in the field of 3 cataclysmic variables.
Ref:	=2004AJ....127..460H
by	HARRISON T.E. , JOHNSON J.J., McARTHUR B.E., BENEDICT G.F., SZKODY P., HOWELL S.B., GELINO D.M.
	Astron. J., 127, 460-468 (2004)
	An astrometric calibration of the M_{V}–P{orb}relationship for cataclysmic variables based on Hubble Space Telescope fine guidance sensor parallaxes.
o	Tables 1, 2: <[HJM2004] WZ Sge Ref N> (Nos 1-5), <[HJM2004] YZ Cnc Ref N> (Nos 1-4), <[HJM2004] RU Peg Ref N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJN2000]
[HJN2000]	(Hansen+Jorgensen+Nagaard-Nielsen+, 1999)= ([HJN2000a]) (Not yet in Simbad)
Write:	<<[HJN2000] C100-N>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	N=4 60mu.m sources observed with a PHT-C camera (C100 detector in the format). Paper I: [HJN99], III: [HJN2000b].
in source:	Ser 159-3
Ref:	=2000A&A...356...83H
by	HANSEN L. , JORGENSEN H.E., NORGAARD-NIELSEN H.U., PEDERSEN K., GOUDFROOIJ P., LINDEN-VORNLE M.J.D.
	Astron. Astrophys., 356, 83-88 (2000)
	ISO far-infrared observations of rich galaxy clusters. II. Sersic 159-03.
o	Table 2: <[HJN2000] C100-N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJN2000a]
[HJN2000a]	(Hansen+Jorgensen+Nagaard-Nielsen+, 1999) (Not yet in Simbad)
*****	Avoid the usage of [HJN2000a], prefer [HJN2000]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJN2000b]
[HJN2000b]	(Hansen+Jorgensen+Norgaard-Nielsen+, 2000) (Not yet in Simbad)
Write:	<<[HJN2000b] ACO 2052 N>>
N:	4
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	ISO observations of ACO 2052. Paper I: [HJN99], II: [HJN2000].
in source:	ACO 2052
Ref:	=2000A&A...362..133H
by	HANSEN L. , JORGENSEN H.E., NORGAARD-NIELSEN H.U., PEDERSEN K., GOUDFROOIJ P., LINDEN-VORNLE M.J.D.
	Astron. Astrophys., 362, 133-137 (2000)
	ISO far-infrared observations of rich galaxy clusters. III. Abell 2029, Abell 2052, Abell 2142.
o	Fig.3, Table 3: <[HJN2000b] ACO 2052 N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJN2003]
[HJN2003]	(Heidt+Jager+Nilsson+, 2003) (Not yet in Simbad)
Write:	<<[HJN2003] aNNa>>
N:	18+18
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	ESO-NTT and VLT telescopes observations of the field of PKS 0537-441.
Ref:	=2003A&A...406..565H
by	HEIDT J. , JAEGER K., NILSSON K., HOPP U., FRIED J.W., SUTORIUS E.
	Astron. Astrophys., 406, 565-577 (2003)
	PKS 0537-441: Extended [OII] emission and a binary QSO?
o	Fig.1: <[FMT92] AN> (No. B2) added. Table 1: <[HJN2003] aNNa> N=18+18.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJN2005]
[HJN2005]	(Huynh+Jackson+Norris, 2005)
Write:	<<[HJN2005] 1.4GHz NNN>>
N:	466
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA 1.4GHz observations of the HDFS. See also [HJN2007] for the 2.5, 5.2 and 8.7GHz catalogs, and ATHDFS.
in source:	NAME HDFS
Ref:	=2005AJ....130.1373H
by	HUYNH M.T. , JACKSON C.A., NORRIS R.P., PRANDONI I.
	Astron. J., 130, 1373-1388 (2005)
	Radio observations of the Hubble Deep Field-South region. II. The 1.4 GHz catalog and source counts.
o	Table 1: <[HJN2005] 1.4GHz NNN> (Nos 1-466) = <ATHDFS JHHMMSS.s+DDMMSSA> N=466.
=E=	Catalogue in electronic form as J/AJ/130/1373
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJN2007]
[HJN2007]	(Huynh+Jackson+Norris+, 2007)
Write:	<<[HJN2007] 2.5GHz NNN>> <<[HJN2007] 5.2GHz NN>> <<[HJN2007] 8.7GHz N>>
N:	149+42+8
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ATCA 2.5, 5.2, and 8.7GHz observations of the HDFS. See also [HJN2005] for the 1.4GHz catalog and ATHDFS.
in source:	NAME HDFS
Ref:	=2007AJ....133.1331H
by	HUYNH M.T. , JACKSON C.A., NORRIS R.P.
	Astron. J., 133, 1331-1344 (2007)
	Radio observations of the Hubble Deep Field-South region. III. The 2.5, 5.2, and 8.7 GHz catalogs and radio source properties.
o	Tables 4, 7: <[HJN2007] 2.5GHz NNN> (Nos 1-149). Tables 5, 8: <[HJN2007] 5.2GHz NN> (Nos 1-42). Tables 6, 9: <[HJN2007] 8.7GHz N> (Nos 1-8). Table 9: <ATHDFS JHHMMSS.s+DDMMSSA> N=463.
=E=	Catalogue in electronic form as <J/AJ/133/1331/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJN99]
[HJN99]	(Hansen+Jorgensen+Nagaard-Nielsen+, 1999)
Write:	<<[HJN99] {S\|H\|V}N>>
N:	3+2+1
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	ISO PHT-C observations. Fig.3: (Nos S1-S3), 3 (IR) sources in ACO 2670. (Nos H1-H2), 2 galaxies in ACO 2670. (No. V), 1 faint radio-source detected with the VLA. Paper II: [HJN2000], III: [HJN2000b]. See also [HW97b].
in source:	ACO 2670
Ref:	=1999A&A...349..406H
by	HANSEN L. , JORGENSEN H.E., NORGAARD-NIELSEN H.U., PEDERSEN K., GOUDFROOIJ P., LINDEN-VORNLE M.J.D.
	Astron. Astrophys., 349, 406-410 (1999)
	ISO far-infrared observations of rich galaxy clusters. I. Abell 2670.
o	Fig.3: cD galaxy = [SEG88] 1, X1 to X3 = [HW97b] 1 to 3.
o	Fig.3: <[HJN99] SN> (Nos S1-S3), <[HJN99] HN> (Nos H1-H2), <[HJN99] V> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJS2019]
[HJS2019]	(Hartley+Jackson+Sluse+, 2019) (Not yet in Simbad)
Write:	<<[HJS2019] HS 0810+2554 AN>>
N:	8
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	European VLBI Network (EVN) and e-MERLIN observations of N=8 lensed components in the images of the gravitationally lensed quasar HS 0810+2554. See also [RHB2002].
in source:	[RHB2002] HS 0810+2554
Ref:	=2019MNRAS.485.3009H
by	HARTLEY P. , JACKSON N., SLUSE D., STACEY H.R., VIVES-ARIAS H.
	Mon. Not. R. Astron. Soc., 485, 3009-3023 (2019)
	Strong lensing reveals jets in a sub-microJy radio-quiet quasar.
o	Fig. 1, Table 5: <[HJS2019] HS 0810+2554 AN> (Nos A1-A2, B1-B2, C1-C2, D1-D2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJS91]
[HJS91]	(Hartmann+Jones+Stauffer+, 1991)= (J) = (J1-)
Write:	<<[HJS91] NNNNA>>
N:	7 among 4872
Object:	PMS* (SIMBAD class: YSO = Young Stellar Object)
Note:	These stars are found in the literature as 'J' or 'J1'. Table 1: N=5 from a survey of about 4600 stars: Nos 507, 644, 665, 4423, 4872. Table 2: Nos 4872A and B. The corresponding 'J2' designation is [GJH92] in SIMBAD
Ref:	=1991AJ....101.1050H
by	HARTMANN L. , JONES B.F., STAUFFER J.R., KENYON S.J.
	Astron. J., 101, 1050-1062 (1991)
	A proper motion survey for pre-main-sequence stars in Taurus-Auriga.
o	Tables 1, 2: <[HJS91] NNNNA> N=7 among 4872 'J NNNN' for authors)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJT2013]
[HJT2013]	(Heida+Jonker+Torres+, 2013)
Write:	<<[HJT2013] ESO 306-003 ULX>>
N:	1
Object:	Poss. ULX (SIMBAD class: ULX_Candidate = Ultra-luminous X-ray Source Candidate)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 observations of N=1 ULX in ESO 306-003.
in source:	ESO 306-3
Ref:	=2013MNRAS.433..681H
by	HEIDA M. , JONKER P.G., TORRES M.A.P., ROBERTS T.P., MINIUTTI G., FABIAN A.C., RATTI E.M.
	Mon. Not. R. Astron. Soc., 433, 681-687 (2013)
	VLT/FORS2 observations of four high-luminosity ULX candidates.
o	<[HJT2013] ESO 306-003 ULX> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HJV94]
[HJV94]	(Hasinger+Johnston+Verbunt, 1994)= (X)
Write:	<<[HJV94] NN>>
N:	21
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations
in source:	NGC 104 = 47 Tuc
Ref:	=1994A&A...288..466H
by	HASINGER G. , JOHNSTON H.M., VERBUNT F.
	Astron. Astrophys., 288, 466-471 (1994)
	Discovery of multiple X-ray sources in 47 Tucanae.
o	Table 1: <[HJV94] NN> (Nos 1-15)
Ref:	=1998A&A...336..895V
by	VERBUNT F. , HASINGER G.
	Astron. Astrophys., 336, 895-901 (1998)
	Nine X-ray sources in the globular cluster 47 Tucanae.
o	Table 2: <[HJV94] NN> (Nos 16-21).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HK
HK	(Hodge+Kennicutt)
Write:	<<HK NGC NNNN NNN>> <<HK UGC NNNN N>> <<HK IC NNNN NNN>> <<HK NGC NNNNA NNN>> <<HK Ho R NN>> <<HK GR N NN>>
N:	10632
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	HII regions in 125 NGC, IC, UGC, Ho, or GR Galaxies. Complete data are presented in this ref. for ten examples: NGC 1232: N=529, NGC 2403: N=606, NGC 3031: N=803, NGC 4254: N=214, NGC 4303: N=289, NGC 4321: N=286, NGC 4535: N=221, NGC 4631: N=96, NGC 6946: N=540, IC 342: N=668. The data for the 115 remaining galaxies are available from the American Institute of Physics Auxiliary Publication Service.
Ref:	=1983AJ.....88..296H
by	HODGE P.W. , KENNICUTT R.C.Jr
	Astron. J., 88, 296-328 (1983)
	An Atlas of H II regions in 125 galaxies.
o	<HK NGC NNNN NNN>, <HK NGC NNNNA NNN>, <HK IC NNNN NNN>, <HK Ho R NN>, <HK GR N NN>, <HK UGC NNNN N>, N=10632
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HK
HK	(Hodge+Kennicutt+)
*****	Avoid the usage of HK, prefer [HKL88]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HKB2002]
[HKB2002]	(Haas+Klass+Bianchi, 2002) (Not yet in Simbad)
Write:	<<[HKB2002] NGC 1569 A>> <<[HKB2002] Arp 244 KN>>
N:	3+2
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Note:	N=3 components (Nos A-C) to NGC 1569. N=2 Knots in APG 244 = The Antennae.
in source:	NGC 1569
in source:	NAME the Antennae
Ref:	=2002A&A...385L..23H
by	HAAS M. , KLAAS U., BIANCHI S.
	Astron. Astrophys., 385, 23-26 (2002)
	The relation of PAH strength with cold dust in galaxies.
o	Fig.2: <[HKB2002] NGC 1569 A> (Nos A-C), <[HKB2002] Arp 244 KN> (Nos K1-K2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKB2009]
[HKB2009]	(Hodge+Krienke+Bellazzini+, 2009)= ([HKB2009a])
Write:	<<[HKB2009] NN>>
N:	82
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST WFPC2 observations of star clusters in M31.
in source:	M 31 = NGC 224
Ref:	=2009AJ....138..770H
by	HODGE P.W. , KRIENKE O.K., BELLAZZINI M., PERINA S., BARMBY P., COHEN J.G., PUZIA T.H., STRADER J.
	Astron. J., 138, 770-779 (2009)
	An HST/WFPC survey of bright young clusters in M31. II. Photometry of less luminous clusters in the fields.
o	Table 1: <[HKB2009] NN> (Nos 1-82).
=E=	Catalogue in electronic form as <J/AJ/138/770/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKB2009a]
[HKB2009a]	(Hodge+Krienke+Bellazzini+, 2009)
*****	Avoid the usage of [HKB2009a], prefer [HKB2009]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKB2009b]
[HKB2009b]	(Heesen+Krause+Beck+, 2009)
Write:	<<[HKB2009b] AN>>
N:	6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA and Effelsberg 100-m telescope 6cm observations of NGC 253. See also [HBK2009].
in source:	NGC 253
Ref:	=2009A&A...506.1123H
by	HEESEN V. , KRAUSE M., BECK R., DETTMAR R.-J.
	Astron. Astrophys., 506, 1123-1135 (2009)
	Cosmic rays and the magnetic field in the nearby starburst galaxy NGC 253. II. The magnetic field structure.
o	Figs 2, 5: <[HKB2009b] AN> (Nos D1-D2, E1-E2, S1-S2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKB2010]
[HKB2010]	(Hodge+Krienke+Bianchi+, 2010)= ([HKB2010a])
Write:	<<[HKB2010] NN>>
N:	86
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST WFPC2 observations of N=86 star clusters in M31.
in source:	M 31 = NGC 224
Ref:	=2010PASP..122..745H
by	HODGE P. , KRIENKE O.K., BIANCHI L., MASSEY P., OLSEN K.
	PASP, 122, 745-752 (2010)
	A photometric catalog of 77 newly recognized star clusters in M31.
o	T.3 : BH05 = M31GC J004030+404530; BH06 = M31GC J004031+404454; DAO 69 = [CCS85] 69; B118D = Bol D118; C410 = [H81] B-410; KHM 540, 566 = KHM31 540, 566; V212 = [V62] 212.
o	Table 3: <[HKB2010] NN> (Nos 1-86).
=E=	Catalogue in electronic form as <J/PASP/122/745/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKB2010a]
[HKB2010a]	(Hodge+Krienke+Bianchi+, 2010)
*****	Avoid the usage of [HKB2010a], prefer [HKB2010]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKB2010b]
[HKB2010b]	(Hanson+Kurtev+Borissova+, 2010)
Write:	<<[HKB2010b] ObjNN>>
N:	11
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	LCO 6.5m Baade telescope PANIC photometry and VLT ISAAC spectroscopy of the dense stellar cluster Mercer 23.
in source:	[MCM2005b] 23
Ref:	=2010A&A...516A..35H
by	HANSON M.M. , KURTEV R., BORISSOVA J., GEORGIEV L., IVANOV V.D., HILLIER D.J., MINNITI D.
	Astron. Astrophys., 516A, 35-35 (2010)
	Obscured clusters. III. Follow-up observations of Mercer 23.
o	Fig. 2, Tables 2-3: <[HKB2010b] ObjNN> (Nos 1-11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKB2011]
[HKB2011]	(Hodge+Krienke+Bianchi, 2011)
Write:	<<[HKB2011] OBNNNWaa>> <<[HKB2011] OBNNNWa'>> <<[HKB2011] OBNNN NN>>
N:	291+48
Object:	HII + UV-Bright star (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=291 nebulae associated with 21 of the van den Bergh OB associations (see [V64]) and N=48 UV-bright stars. Use of HST (GO-11079) and NOAO Local Group Survey data in M31.
in source:	M 31 = NGC 224
Ref:	=2011PASP..123..649H
by	HODGE P.W. , KRIENKE O.K., BIANCHI L.
	PASP, 123, 649-658 (2011)
	A morphological study of UV-bright stars and emission nebulae in a selection of star formation regions in M31.
o	Table 1: <[HKB2011] OBNNNWaa>, <[HKB2011] OBNNNWa'> N=291. Table A1: <[HKB2011] OBNNN NN > N=48.
=E=	Catalogue in electronic form as J/PASP/123/649
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKC2000]
[HKC2000]	(Haas+Klaas+Coulson+, 2000)
Write:	<<[HKC2000] KN>>
N:	2
Object:	Knot (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	N=2 bright 850 mu.m emission knots observed on the SCUBA maps in NGC 4038/39 system.
in source:	NAME the Antennae
Ref:	=2000A&A...356L..83H
by	HAAS M. , KLAAS U., COULSON I., THOMMES E., XU C.
	Astron. Astrophys., 356, 83-87 (2000)
	The cold dust concentrations in the colliding galaxies NGC 4038/39.
o	Fig.1: radio peaks 2, 3, 4 = [HV86] 2, 3, 4.
o	Fig.1, Table 1: <[HKC2000] KN> (Nos K1-K2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKD2003]
[HKD2003]	(Haverkorn+Katgert+De Bruyn, 2003)= ([HKD2003a])
Write:	<<[HKD2003] NN>>
N:	13
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	WSRT observations. N=13 extragalactic sources in the Auriga region.
Ref:	=2003A&A...403.1031H
by	HAVERKORN M. , KATGERT P., DE BRUYN A.G.
	Astron. Astrophys., 403, 1031-1044 (2003)
	Multi-frequency polarimetry of the Galactic radio background around 350 MHz. I. A region in Auriga around l = 161°, b = 16°.
o	Table 3: <[HKD2003] NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKD2003a]
[HKD2003a]	(Haverkorn+Katgert+De Bruyn, 2003)
*****	Avoid the usage of [HKD2003a], prefer [HKD2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKD2003b]
[HKD2003b]	(Haverkorn+Katgert+De Bruyn, 2003)
Write:	<<[HKD2003b] NN>>
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	WSRT observations. N=12 extragalactic sources in the Horologium region, close to a ring-like structure in polarization.
Ref:	=2003A&A...404..233H
by	HAVERKORN M. , KATGERT P., DE BRUYN A.G.
	Astron. Astrophys., 404, 233-247 (2003)
	Multi-frequency polarimetry of the Galactic radio background around 350 MHz II. A region in Horologium around l = 137°, b = 7°.
o	Table 2: <[HKD2003b] NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKD2016]
[HKD2016]	(Husser+Kamann+Dreizler+, 2016)
Write:	<<[HKD2016] NNNNNNNN>>
N:	2758
Object:	* (SIMBAD class: Star)
Note:	VLT MUSE observations of N=2758 stars in the globular cluster NGC 6397.
in source:	NGC 6397
Ref:	=2016A&A...588A.148H
by	HUSSER T.-O. , KAMANN S., DREIZLER S., WENDT M., WULFF N., BACON R., WISOTZKI L., BRINCHMANN J., WEILBACHER P.M., ROTH M.M., MONREAL-IBERO A.
	Astron. Astrophys., 588A, 148-148 (2016)
	MUSE crowded field 3D spectroscopy of over 12 000 stars in the globular cluster NGC 6397.
o	<[HKD2016] NNNNNNNN> N=2758 among (Nos 11000001-24000582).
=E=	Catalogue in electronic form as J/A+A/588/A148
Details on Acronym: [HKE2011]
[HKE2011]	(Hofner+Kurtz+Ellingsen+, 2011)
Write:	<<[HKE2011] IRAS HHMMm+DDMM A>>
N:	10
Object:	(cm) (SIMBAD class: cmRad = Centimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	EVLA 1.3cm observations of N=10 continuum sources toward IRAS 18151-1208, IRAS 18182-1433, IRAS 18345-0641, IRAS 18470-0044 and IRAS 19012+0536.
in source:	IRAS 18182-1433
in source:	IRAS 18345-0641
in source:	IRAS 18470-0044
in source:	IRAS 19012+0536
Ref:	=2011ApJ...739L..17H
by	HOFNER P. , KURTZ S., ELLINGSEN S.P., MENTEN K.M., WYROWSKI F., ARAYA E.D., LOINARD L., RODRIGUEZ L.F., CESARONI R.
	Astrophys. J., 739L, 17 (2011)
	Expanded very large array continuum observations toward hot molecular core candidates.
o	Table 2: <[HKE2011] IRAS HHMMm+DDMM A> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKE2013]
[HKE2013]	(Hermanowicz+Kennicutt+Eldridge, 2013)
Write:	<<[HKE2013] NGC NNNN NNN>>
N:	279+647+201+431+693+518+417
Object:	Star Forming Region (SIMBAD class: StarFormingReg = Star Forming Region)
Note:	Study of Hα/FUV flux ratios of star-forming regions within seven nearby spiral galaxies.
in source:	NGC 628
in source:	NGC 2403
in source:	NGC 300
in source:	NGC 3031
in source:	NGC 5236
in source:	NGC 5457
in source:	NGC 7793
Ref:	=2013MNRAS.432.3097H
by	HERMANOWICZ M.T. , KENNICUTT R.C., ELDRIDGE J.J.
	Mon. Not. R. Astron. Soc., 432, 3097-3116 (2013)
	Hα to FUV ratios in resolved star-forming region populations of nearby spiral galaxies.
o	Table 3: <[HKE2013] NGC NNNN NNN> N=279+647+201+431+693+518+417.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKF2002]
[HKF2002]	(Hornoch+Kusnirak+Foley+, 2002)
Write:	<<[HKF2002] JHHMMSS.s+DDMMSS>>
N:	1
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Stat:	is completely incorporated in Simbad
Note:	Lelekovice and Lick observations. Discovery of a new nova in M 31.
in source:	M 31 = NGC 224
Ref:	=2002IAUC.7970....2H
by	HORNOCH K. , KUSNIRAK P., FOLEY R.J., JHA S., PAPENKOVA M., FILIPPENKO A.V.
	IAU Circ., 7970, 2-None (2002)
	Nova in M31.
o	<[HKF2002] JHHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HKK
HKK	(Huchtmeier+Karachentsev+Karachentseva)= (HKK97)
Write:	<<HKK LNNN>>
N:	26
Object:	Dwarf G (SIMBAD class: Galaxy)
Note:	N=26 new dwarf galaxies candidates. See also [KK98a]
Ref:	=1997A&A...322..375H
by	HUCHTMEIER W.K. , KARACHENTSEV I.D., KARACHENTSEVA V.E.
	Astron. Astrophys., 322, 375-380 (1997)
	HI-search for nearby dwarf galaxies.
o	Table 1, col(4): <HKK LNNN> N=26 among (Nos L8-L41 and L147-L151).
Origin	of the Acronym: L (1999PASA...16...48R)
Details on Acronym: [HKK2001]
[HKK2001]	(Higgs+Kerton+Knee, 2001)
Write:	<<[HKK2001] HI Cloud>> <<[HKK2001] Knot NN>>
N:	1+10
Object:	Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Note:	N=1 HI cloud near the galactic plane, with N=10 HI knots. See also 71P, 72P.
Ref:	=2001AJ....122.3155H
by	HIGGS L.A. , KERTON C.R., KNEE L.B.G.
	Astron. J., 122, 3155-3170 (2001)
	A peculiar intermediate-velocity hydrogen cloud near the galactic plane.
o	<[HKK2001] HI Cloud> N=1. Table 3: <[HKK2001] Knot NN> (Nos 1-10). Table 4: <71P NNN> (Nos 1-106). Table 5: <72P NN> (Nos 1-56).
=E=	Catalogue in electronic form as J/AJ/122/3155
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKK2009]
[HKK2009]	(Huchtmeier+Karachentsev+Karachentseva, 2009)
Write:	<<[HKK2009] dJHHMM+DDMM>> <<[HKK2009] dHHMM+DDMM>> (not recognised by Simbad, but found in literature)
N:	57
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Effelsberg 100m telescope observations of galaxies in nearby groups.
in source:	NAME Local Supercluster
Ref:	=2009A&A...506..677H
by	HUCHTMEIER W.K. , KARACHENTSEV I.D., KARACHENTSEVA V.E.
	Astron. Astrophys., 506, 677-680 (2009)
	HI-observations of dwarf galaxies in the Local Supercluster.
o	Tables 1-3: <[HKK2009] dJHHMM+DDMM> N=12+12+57.
=E=	Catalogue in electronic form as J/A+A/506/677
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKK2011]
[HKK2011]	(Hayashi+Kodama+Tadaki+, 2011)
Write:	<<[HKK2011] NN>>
N:	16
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Subaru Suprime-Cam and MOIRCS observations of N=16 [OII] emitters in the central region of the cluster XMMXCS J2215.9-1738.
in source:	XMMXCS J2215.9-1738 = ClG J2215-1738
Ref:	=2011MNRAS.415.2670H
by	HAYASHI M. , KODAMA T., KOYAMA Y., TADAKI K.-I., TANAKA I.
	Mon. Not. R. Astron. Soc., 415, 2670-2687 (2011)
	Properties of star-forming galaxies in a cluster and its surrounding structure at z = 1.46.
o	Tables 3-4: <[HKK2011] NN> (Nos 1-16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKK2017]
[HKK2017]	(Hayashi+Kodama+Kohno+, 2017)
Write:	<<[HKK2017] ALMA.B3.NN>>
N:	17
Object:	G (SIMBAD class: Galaxy)
Note:	ALMA cycle 3 CO(2-1) observations of N=17 galaxies in the XMMXCS J2215.9-1738 galaxy cluster. See also <[HTK2018]>.
in source:	XMMXCS J2215.9-1738
Ref:	=2017ApJ...841L..21H
by	HAYASHI M. , KODAMA T., KOHNO K., YAMAGUCHI Y., TADAKI K.-I., HATSUKADE B., KOYAMA Y., SHIMAKAWA R., TAMURA Y., SUZUKI T.L.
	Astrophys. J., 841L, 21-21 (2017)
	Evolutionary phases of gas-rich galaxies in a galaxy cluster at z = 1.46.
o	Table 1: <[HKK2017] ALMA.B3.NN> (Nos 1-17).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HKK97
HKK97	(Huchtmeier+Karachentsev+Karachentseva, 1997)
*****	Avoid the usage of HKK97, prefer HKK
Origin	of the Acronym: L (2003AJ....126.1707G)
Details on Acronym: HKL
HKL	(Henning+Klein+Launhardt+)
*****	Avoid the usage of HKL, prefer [HKL98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HKL2017]
[HKL2017]	(Hollyhead+Kacharov+Lardo+, 2017)
Write:	<<[HKL2017] NNNN>>
N:	34
Object:	* (SIMBAD class: Star)
Note:	VLT FORS2 spectroscopic observations of N=34 stars in the SMC stellar cluster Cl Lindsay 1. See also [HLK2018].
in source:	Magellanic Clouds:SMC:Cl Lindsay 1 = Cl Lindsay 1
Ref:	=2017MNRAS.465L..39H
by	HOLLYHEAD K. , KACHAROV N., LARDO C., BASTIAN N., HILKER M., REJKUBA M., KOCH A., GREBEL E.K., GEORGIEV I.
	Mon. Not. R. Astron. Soc., 465L, 39-43 (2017)
	Evidence for multiple populations in the intermediate-age cluster Lindsay 1 in the SMC.
o	Table 1: <[HKL2017] NNNN> N=34 among (Nos 8-5589).
=E=	Catalogue in electronic form as <J/MNRAS/465/L39/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKL88]
[HKL88]	(Hodge+Kennicutt+Lee, 1988)= (HK)
Write:	<<[HKL88] NNN>>
N:	110
Object:	HII (SIMBAD class: HIIReg = HII Region)
in source:	NGC 6822
Ref:	=1988PASP..100..917H
by	HODGE P. , KENNICUTT R.C.Jr, LEE M.G.
	Publ. Astron. Soc. Pac., 100, 917-934 (1988)
	The HII regions of NGC 6822. I. An atlas of 157 HII regions.
o	Table IV: <[HKL88] NNN> N=110
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKL89]
[HKL89]	(Hummel+Krause+Lesch, 1989)
Write:	<<[HKL89] NN>> <<[HKL89] A>>
N:	10+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 2: Background sources at 1.49GHz in the field of NGC 4258.
Ref:	=1989A&A...211..266H
by	HUMMEL E. , KRAUSE M., LESCH H.
	Astron. Astrophys., 211, 266-274 (1989)
	Linearly polarized radioemission from the anomalous arms in NGC 4258 (M 106).
o	Table 2: <[HKL89] NN> (Nos 1-10), <[HKL89] A> (No. A).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKL98]
[HKL98]	(Henning+Klein+Launhardt+, 1998)= (HKL) = (IRS)
Write:	<<[HKL98] IRS N>>
N:	5
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	ISO SWS/LWS and CAM observations.
in source:	NAME M 17N
Ref:	=1998A&A...332.1035H
by	HENNING T. , KLEIN R., LAUNHARDT R., LEMKE D., PFAU W.
	Astron. Astrophys., 332, 1035-1043 (1998)
	The molecular cloud core M17-North: ISO spectroscopy and IR/mm continuum mapping.
o	Fig.5: <[HKL98] IRS N> (Nos 1-2).
Ref:	=1999A&A...343L..53K
by	KLEIN R. , HENNING T., CESARSKY D.
	Astron. Astrophys., 343, 53-56 (1999)
	The molecular cloud core M17-North: New ISOCAM observations.
o	Table 1: <[HKL98] IRS N> (Nos 3-5) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKM96]
[HKM96]	(Herbstmeier+Kalberla+Mebold+, 1996)
Write:	<<[HKM96] NN>>
N:	27
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=27 continuum point sources.
in source:	NAME Draco Nebula
Ref:	=1996A&AS..117..497H
by	HERBSTMEIER U. , KALBERLA P.M.W., MEBOLD U., WEILAND H., SOUVATZIS I., WENNMACHER A., SCHMITZ J.
	Astron. Astrophys., Suppl. Ser., 117, 497-518 (1996)
	Single-dish and aperture synthesis H I observations towards the Draco nebula. I. The data.
o	Table 5: <[HKM96] NN> (Nos 1-27)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKM97]
[HKM97]	(Hurley+Kouveliotou+Marshall+, 1997)
Write:	<<[HKM97] AN>>
N:	4
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ASCA SIS observations: N=4 X-ray sources in the error box of GRB 970616. See also [GVM97].
Ref:	=1997IAUC.6687....1H
by	HURLEY K. , KOUVELIOTOU C., MARSHALL F., MURAKAMI T., FUJIMOTO R., UEDA Y., SHIBATA R., GALAMA T., BROADHURST T., FRYE B., VAN PARADIJS J.
	IAU Circ., 6687, 1-None (1997)
	GRB 970616.
o	Numbering 'AN' for the 4 ASCA sources is found in 1999A&AS..138..455G
o	<[HKM97] AN> (Nos A1-A4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKM99]
[HKM99]	(Hirano+Kamazaki+Mikami+, 1999)
Write:	<<[HKM99] B1-a>> <<[HKM99] B1-aW>> <<[HKM99] B1-IRS>>
N:	4+2+1
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=4 ammonia condensations 'B1-a' to 'B1-d' in Barnard 1 cloud. N=2 smm peaks in B1-b condensation 'B1-bN' and 'B1-bS'.
in source:	Barnard 1
Ref:	=1999sf99..R....181H
by	HIRANO N. , KAMAZAKI T., MIKAMI H., OHASHI N., UMEMOTO T.
	Proc. Star Formation 1999, 181-182 (1999)
	Discovery of two extreme young protostars in Barnard 1.
o	Fig.1: <[HKM99] B1-a> (Nos B1-a, B1-b), <[HKM99] B1-bW> (Nos B1-bN, B1-bS), <[HKM99] B1-IRS> N=1.
Ref:	=2002ApJ...574..822M
by	MATTHEWS B.C. , WILSON C.D.
	Astrophys. J., 574, 822-833 (2002)
	Magnetic fields in star-forming molecular clouds. V. Submillimeter polarization of the Barnard 1 dark cloud.
o	First reference in 1999, Proc. Star formation, ed. T. Nakamoto (Nagano): Discovery of two extreme young protostars in Barnard 1.
o	Fig.1: <[HKM99] B1-a> (Nos B1-c, B1-d) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKN2006]
[HKN2006]	(Hatano+Kadowaki+Nakajima+, 2006)
Write:	<<[HKN2006] OB NNN>> <<[HKN2006] HAeBe NNN>> <<[HKN2006] OC N>> <<[HKN2006] HC N>>
N:	559+127+4+6
Object:	* (SIMBAD class: Star)
Note:	IRFS 1.4m telescope at the South African Astronomical Observatory (Sutherland) NIR observations of LHA 120-N 11: N=559 OB stars, N=127 Herbig Ae-Be stars, and N=4+6 concentrations of OB and HAeBe stars.
in source:	Magellanic Clouds:LMC:LHA 120-N 11 = LHA 120-N 11
Ref:	=2006AJ....132.2653H
by	HATANO H. , KADOWAKI R., NAKAJIMA Y., TAMURA M., NAGATA T., SUGITANI K., TANABE T., KATO D., KURITA M., NISHIYAMA S., BABA D., ISHIHARA A., SATO S.
	Astron. J., 132, 2653-2664 (2006)
	Near-infrared observations of N11 in the Large Magellanic Cloud: triggered star formation around the periphery of LH 9.
o	Table 1: <[HKN2006] OB NNN> (Nos 1-559). Table 2: <[HKN2006] HAeBe NNN> (Nos 1-137). Table 3: <[HKN2006] OC N> (Nos 1-4), <[HKN2006] HC N> (Nos 1-6).
=E=	Catalogue in electronic form as J/AJ/132/2653
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKP2005]
[HKP2005]	(Hoyos+Koo+Phillips+, 2005)
Write:	<<[HKP2005] D-NN>> <<[HKP2005] TK-N>>
N:	14+3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Discovery of luminous, metal-poor star-forming galaxies from the DEEP2 and TKRS surveys.
Ref:	=2005ApJ...635L..21H
by	HOYOS C. , KOO D.C., PHILLIPS A.C., WILLMER C.N.A., GUHATHAKURTA P.
	Astrophys. J., 635, 21-24 (2005)
	The DEEP2 galaxy redshift survey: discovery of luminous, metal-poor star-forming galaxies at redshifts z ~ 0.7.
o	Table 1: <[HKP2005] D-NN> (Nos D-1 to D-14), <[HKP2005] TK-N> (Nos TK-1 to TK-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HKPN
HKPN	(Hurley-Keller+, PN)
Write:	<<HKPN M31 NNN>> <<HKPN M32 N>>
N:	135+8
Object:	Poss. PN (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
Stat:	is completely incorporated in Simbad
Note:	Observations at the Case Western Reserve University Burrell Schmidt to search for PN in M 31 and M32.
in source:	M 31 = NGC 224
in source:	M 32 = NGC 221
Ref:	=2004ApJ...616..804H
by	HURLEY-KELLER D. , MORRISON H.L., HARDING P., JACOBY G.H.
	Astrophys. J., 616, 804-820 (2004)
	Planetary nebula kinematics in M31.
o	Table 1: <HKPN M31 NNN> (Nos 1-135). Table 2: <HKPN M32 N> (Nos 1-8).
=E=	Catalogue in electronic form as J/ApJ/616/804
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HKR2008]
[HKR2008]	(Hamann+Kaplan+Rodriguez Hidalgo+, 2008) (Not yet in Simbad)
Write:	<<[HKR2008] SDSS J105400.40+034801.2 abs N.NNNN>>
N:	1
Object:	DLA
Note:	Spectroscopic observations of the QSO SDSS J105400.40+034801.2.
Ref:	=2008MNRAS.391L..39H
by	HAMANN F. , KAPLAN K.F., RODRIGUEZ HIDALGO P., PROCHASKA J.X., HERBERT-FORT S.
	Mon. Not. R. Astron. Soc., 391L, 39-43 (2008)
	Emergence of a quasar outflow.
o	Fig.1: <[HKR2008] SDSS J105400.40+034801.2 abs N.NNNN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKR2018]
[HKR2018]	(Hare+Kargaltsev+Rangelov, 2018) (Not yet in Simbad)
Write:	<<[HKR2018] XNN>> <<[HKR2018] JDDD.dddddd+DD.dddddd>>
N:	15+12
Object:	(X) + (NIR) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=15 X-ray sources extracted from Chandra ACIS archival data in the cluster GLIMPSE C01. HST WFC3 observations of N=12 NIR sources, potential counterparts to the X-ray sources.
in source:	GLIMPSE C01
Ref:	=2018ApJ...865...33H
by	HARE J. , KARGALTSEV O., RANGELOV B.
	Astrophys. J., 865, 33-33 (2018)
	Chandra X-Ray Observatory and Hubble Space Telescope observations of the intermediate-age cluster GLIMPSE-C01.
o	Fig. 2, Table 2: <[HKR2018] XNN> (Nos X1-X15). Table 3: <[HKR2018] JDDD.dddddd+DD.dddddd> N=12.
=E=	Catalogue in electronic form as <J/ApJ/865/33/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKS2001]
[HKS2001]	(Hrivnak+Kwok+Su, 2001) (Not yet in Simbad)
Write:	<<[HKS2001] IRAS 16594-4656 Arc N>> <<[HKS2001] IRAS 20028+3910 Arc N>>
N:	4+3
Object:	Arc (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST WFPC2 images of IRAS 16594-4656 and IRAS 20028+3910 Discover of circumstellar arcs.
in source:	IRAS 16594-4656
in source:	IRAS 20028+3910
Ref:	=2001AJ....121.2775H
by	HRIVNAK B.J. , KWOK S., SU K.Y.L.
	Astron. J., 121, 2775-2780 (2001)
	The discovery of circumstellar arcs around two bipolar proto-planetary nebulae.
o	Fig.1: <[HKS2001] IRAS 16594-4656 Arc N> (Nos 1-4). Fig.2: <[HKS2001] IRAS 20028+3910 Arc N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKS2011]
[HKS2011]	(Hirota+Kuno+Sato+, 2011)
Write:	<<[HKS2011] NN>>
N:	26
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	Nobeyama Millimeter Array 12CO(1-0) and 13CO(1-0) observations of a spiral arm of IC 342.
in source:	IC 342
Ref:	=2011ApJ...737...40H
by	HIROTA A. , KUNO N., SATO N., NAKANISHI H., TOSAKI T., SORAI K.
	Astrophys. J., 737, 40 (2011)
	Giant molecular clouds in the spiral arm of IC 342.
o	Fig. 4, Table 2: <[HKS2011] NN> (Nos 1-26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKS2013]
[HKS2013]	(Hodge+Karim+Smail+, 2013)
Write:	<<[HKS2013] ALESS NNN.NN>>
N:	99+32
Object:	smm G (SIMBAD class: Galaxy)
Note:	ALMA Cycle 0 870µm survey of 126 submillimeter sources from the LABOCA ECDFS Submillimeter Survey (LESS). The ALESS SMG catalog includes the main sample of 99 submillimeter galaxies and a supplementary sample of 32 submillimeter galaxies.
in source:	NAME ECDFS
Ref:	=2013ApJ...768...91H
by	HODGE J.A. , KARIM A., SMAIL I., SWINBANK A.M., WALTER F., BIGGS A.D., IVISON R.J., WEISS A., ALEXANDER D.M., BERTOLDI F., BRANDT W.N., CHAPMAN S.C., COPPIN K.E.K., COX P., DANIELSON A.L.R., DANNERBAUER H., DE BREUCK C., DECARLI R., EDGE A.C., GREVE T.R., KNUDSEN K.K., MENTEN K.M., RIX H.-W., SCHINNERER E., SIMPSON J.M., WARDLOW J.L., VAN DER WERF P.
	Astrophys. J., 768, 91 (2013)
	An ALMA survey of submillimeter galaxies in the Extended Chandra Deep Field South: source catalog and multiplicity.
o	Tables 3-4: <[HKS2013] ALESS NNN.NN> = <ALESS JHHMMSS.ss+DDMMSS.s>, N=99+32.
=E=	Catalogue in electronic form as <J/ApJ/768/91/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKS2019]
[HKS2019]	(Hanaoka+Kaneda+Suzuki+, 2019)
Write:	<<HKS2019 ENNN>> <<HKS2019 EWNN>>
N:	141+38
Object:	IR Bubble (SIMBAD class: Bubble)
Stat:	is completely incorporated in Simbad
Note:	N=141+38 IR bubbles in the outer and high-latitude inner Galactic regions respectively. Use of AKARI all-sky survey data in the mid-IR wavelengths.
Ref:	=2019PASJ...71....6H
by	HANAOKA M. , KANEDA H., SUZUKI T., KOKUSHO T., OYABU S., ISHIHARA D., KOHNO M., FURUTA T., TSUCHIKAWA T., SAITO F.
	PASJ, 71, 6 (2019)
	A systematic study of Galactic infrared bubbles along the Galactic plane with AKARI and Herschel.
o	Fig. 12, Tables 2-4: <[HKS2019] ENNN> (Nos E1-E141), <[HKS2019] EWNN> (Nos EN1-EN22, ES1-ES16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKS94]
[HKS94]	(Hodge+Kennicutt+Strobel, 1994)
Write:	<<[HKS94] NN>>
N:	25
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
in source:	Sextans A = DDO 75
Ref:	=1994PASP..106..765H
by	HODGE P. , KENNICUTT R.C., STROBEL N.
	Publ. Astron. Soc. Pac., 106, 765-769 (1994)
	The H II regions of Sextans A.
o	Table 1: <[HKS94] NN> N=25
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKT2006]
[HKT2006]	(Hudaverdi+Kunieda+Tanaka+, 2006)
Write:	<<[HKT2006] A NNNN NN>>
N:	56+32
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton observations of ACO 194 and ACO 1060.
in source:	ACO 194
in source:	ACO 1060
Ref:	=2006PASJ...58..931H
by	HUDAVERDI M. , KUNIEDA H., TANAKA T., HABA Y., FURUZAWA A., TAWARA Y., ERCAN E.N.
	PASJ, 58, 931-943 (2006)
	Overdensity of X-ray sources in the field of two nearby clusters of galaxies: XMM-Newton view of A 194 and A 1060.
o	Table 6: <[HKT2006] A 194 NN> (Nos 1-56). Table 7: <[HKT2006] A 1060 NN> (Nos 1-32).
=E=	Catalogue in electronic form as J/PASJ/58/931
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKT95]
[HKT95]	(Hopp+Kuhn+Thiele+, 1995)
Write:	<<[HKT95] A NNNN-NNN>> <<[HKT95] AA NNNNA>> <<[HKT95] AAN NNN>> <<[HKT95] AAN KOW NNN>> <<[HKT95] ACO 2151 NNNN>> <<[HKT95] AAA A NNNN-NNN>> <<[HKT95] AAA AA NNNNA>> <<[HKT95] AAA AAN NNN>> <<[HKT95] AAA AAN KOW NNN>> <<[HKT95] AAA ACO 2151 NNNN>>
Object:	G (SIMBAD class: Galaxy)
Note:	The formats are contructed as follows: 'A NNNN-NNN' can be 'O NNNN-NNN' or 'B NNNN-NNN': 'O NNNN-NNN': 'NNNN' stands for the 'old' Palomar blue plates Sky Survey, while 'NNN' is a running number. 'B NNNN-NNN': Same system with B plate of the 'new' POSS-II. 'AA NNNNA' where 'AA' stands for 'HN': galaxies taken from the overlays of the 'old' Palomar Sky Survey refering to an old list of galaxies from Havard. 'AAN NNN' and 'AAN KOW NNN': for VN2, VN4, VN8, and KOW fields used by the authors to identifies the plates of the Calar Alto 3.5m Telescope. 'ACO 2151 NNNN': for an internal running number on a 3.5m plate towards the ACO cluster 2151. 'AAA' before each format for the letters 'N' or 'NN' or 'NNN': 'N' refers to neighbor galaxy not in the original list, but observed with the same slit setting of the spectrograph, so the authors got a redshift. In few cases, we had even 2 or 3 additional galaxies on the slit, adding 'NN' or 'NNN' before the neighbor galaxy.
Ref:	=1995A&AS..109..537H
by	HOPP U. , KUHN B., THIELE U., BIRKLE K., ELSAESSER H., KOVACHEV B.
	Astron. Astrophys., Suppl. Ser., 109, 537-549 (1995)
	A redshift survey for faint galaxies towards voids of galaxies.
o	Table 10: <[HKT95] O NNNN-NNN>, <[HKT95] N O NNNN-NNN>, <[HKT95] HN NNNN>, <[HKT95] VN2 NNN>, <[HKT95] VN4 NNN>, <[HKT95] VN8 NNN>, <[HKT95] VN2 KOW NNN>, <[HKT95] N VN2 NNN>, <[HKT95] N VN4 NNN>, <[HKT95] ACO 2151 NNNN>, N=160
Ref:	=1997A&A...318..405K
by	KUHN B. , HOPP U., ELSAESSER H.
	Astron. Astrophys., 318, 405-415 (1997)
	Results of a search for faint galaxies in voids.
o	Table 1: <[HKT95] AA A NNNN-NNN> format added, the letters 'AA A' standing for 'NN O'
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HKV
HKV	(Hrivnak+Kwok+Volk) (Not yet in Simbad)
Write:	<<HKV N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	Protoplanetary nebula IRAS 18095+2704.
Ref:	=1988ApJ...331..832H
by	HRIVNAK B.J. , KWOK S., VOLK K.M.
	Astrophys. J., 331, 832-837 (1988)
	The high-latitude F supergiant IRAS 18095+2704: a proto-planetary nebula.
o	<HVK N> (No. 1).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HKV86]
[HKV86]	(Hummel+Kotanyi+Van Gorkom, 1986)
Write:	<<[HKV86] Gal A>> <<[HKV86] Knot A>> <<[HKV86] Background NN>> <<[HKV86] Component N>>
N:	4+3+12+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio observations of the field of NGC 4410 interacting pair.
in source:	NGC 4410
Ref:	=1986A&A...155..161H
by	HUMMEL E. , KOTANYI C.G., VAN GORKOM J.H.
	Astron. Astrophys., 155, 161-168 (1986)
	NGC 4410a/b : a strong radio source associated with interacting galaxies.
o	Fig.1, Table 3: <[HKV86] Gal A> (Nos A-D). Table 5: <[HKV86] Knot A> (Nos E-G). Table 2: <[HKV86] Background NN> (Nos 1-12). Table 5: <[HKV86] Component N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKW2012]
[HKW2012]	(Hibon+Kashikawa+Willott+, 2012)
Write:	<<[HKW2012] D33-LAE N>> <<[HKW2012] D41-LAE N>>
N:	14 (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	Subaru SuprimeCam narrow-badn observations of two fields (D33 and D41) covered by the CFHT-LS and the WIRDS.
Ref:	=2012ApJ...744...89H
by	HIBON P. , KASHIKAWA N., WILLOTT C., IYE M., SHIBUYA T.
	Astrophys. J., 744, 89 (2012)
	Search for z ~ 7 Lyα emitters with the Suprime-Cam at the Subaru telescope.
o	Table 2: <[HKW2012] D33-LAE N> (Nos 1-6), Table 3: <[HKW2012] D41-LAE N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKW2014]
[HKW2014]	(Hendricks+Koch+Walker+, 2014)
Write:	<<[HKW2014] NNN>>
N:	353
Object:	* (SIMBAD class: Star)
Note:	VLT FLAMES GIRAFFE observation of N=353 stars in the Fornax dwarf spheroidal galaxy.
in source:	NAME Fornax dSph
Ref:	=2014A&A...572A..82H
by	HENDRICKS B. , KOCH A., WALKER M., JOHNSON C.I., PENARRUBIA J., GILMORE G.
	Astron. Astrophys., 572A, 82-82 (2014)
	Insights from the outskirts: Chemical and dynamical properties in the outer parts of the Fornax dwarf spheroidal galaxy.
o	Tables 1-2: <[HKW2014] NNN> N=353 among (Nos 2-431).
=E=	Catalogue in electronic form as <J/A+A/572/A82/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKW2016]
[HKW2016]	(Hargis+Kimmig+Willman+, 2016)
Write:	<<[HKW2016] DDD.dddddd+DD.dddddd>>
N:	411
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	MMT Hectochelle spectroscopic observations of N=411 stars in the field of the Hydra I overdensity.
in source:	NAME Hydra I overdensity
Ref:	=2016ApJ...818...39H
by	HARGIS J.R. , KIMMIG B., WILLMAN B., CALDWELL N., WALKER M.G., STRADER J., SAND D.J., GRILLMAIR C.J., YOON J.H.
	Astrophys. J., 818, 39 (2016)
	Evidence that Hydra I is a tidally disrupting Milky Way dwarf galaxy.
o	Table 2: <[HKW2016] DDD.dddddd+DD.dddddd> N=411.
=E=	Catalogue in electronic form as J/ApJ/818/39
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKY2018]
[HKY2018]	(Hatsukade+Kohno+Yamaguchi+, 2018)= (ASAGAO)
Write:	<<[HKY2018] NN>>
N:	45
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	ALMA band 6 observations of N=45 sources in the GOODS South field, as part of the Alma twenty-Six Arcmin² survey of GOODS-South At One-millimeter (ASAGAO).
in source:	NAME GOODS South Field
Ref:	=2018PASJ...70..105H
by	HATSUKADE B. , KOHNO K., YAMAGUCHI Y., et al.
	PASJ, 70, 105 (2018)
	ALMA twenty-six arcmin^{2} survey of GOODS-S at one millimeter (ASAGAO): Source catalog and number counts.
o	Figs 6+10, Table 3: <[HKY2018] NN> (Nos 1-45).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HKZ2015]
[HKZ2015]	(Hyde+Keller+Zucker+, 2015)
Write:	<<[HKZ2015] NNN>>
Object:	* (SIMBAD class: Star)
Note:	AAT AAOmega observations of N=106 highly likely members of the Sagittarius stream.
in source:	NAME Sgr Stream
Ref:	=2015ApJ...805..189H
by	HYDE E.A. , KELLER S., ZUCKER D.B., IBATA R., SIEBERT A., LEWIS G.F., PENARRUBIA J., IRWIN M., GILMORE G., LANE R.R., KOCH A., CONN A.R., DIAKOGIANNIS F.I., MARTELL S.
	Astrophys. J., 805, 189 (2015)
	Selecting Sagittarius: identification and chemical characterization of the Sagittarius stream.
o	Table 2: <[HKZ2015] NNN> (Nos 1-106).
=E=	Catalogue in electronic form as <J/ApJ/805/189/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HL
HL	(Haro+Luyten)
Write:	<<HL CCC NN>>
N:	1
Object:	WD (SIMBAD class: WhiteDwarf = White Dwarf)
Ref:	=1961BOTT....3...35H
by	HARO G. , LUYTEN W.J.
	Bol. Obs. Tonantz. Tacub., 3, 35-35 (1961)
	Nueva Estrella enana Blanca en las nubes obscuras del Toro.
o	part no 21
o	<HL TAU 76>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HL
HL	(Hartigan+Lada)
*****	Avoid the usage of HL, prefer [HL85]
Origin	of the Acronym: L (1991A&A...241..589G,1999AJ....118..558K)
Details on Acronym: HL
HL	(Hodge+Lee)
*****	Avoid the usage of HL, prefer [HL90]
Origin	of the Acronym: L (1993AJ....106.1448Y,1998AJ....116.2363W)
Details on Acronym: HL
HL	(Hodapp+Ladd)
*****	Avoid the usage of HL, prefer [HL95]
Origin	of the Acronym: L (2008MNRAS.387..954D)
Details on Acronym: HL
HL	(Hodge+Lee+)
*****	Avoid the usage of HL, prefer [HLK89]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HL
HL	(HL Tau)
*****	Avoid the usage of HL, prefer [MRB88]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HL
HL	(Haro+Luyten)
*****	Avoid the usage of HL, prefer PHL
Details on Acronym: [HL2001]
[HL2001]	(Henden+Landolt, 2001)
Write:	<<[HL2001] N>>
N:	5
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=5 comparison stars in the field of WZ Sge. See also [KK64].
Ref:	=2001IBVS.5166....1H
by	HENDEN A.A. , LANDOLT A.U.
	IAU Inform. Bull. Var. Stars, 5166, 1-None (2001)
	Photometry of stars near WZ Sge.
o	<[HL2001] N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HL2008]
[HL2008]	(Hwang+Lee, 2008)
Write:	<<[HL2008] NNNNNN>>
N:	2224
Object:	Star Cluster (SIMBAD class: Cluster* = Cluster of Stars)
Note:	HST ACS observations of M 51 to search for star clusters.
in source:	M 51 = NGC 5194
Ref:	=2008AJ....135.1567H
by	HWANG N. , LEE M.G.
	Astron. J., 135, 1567-1579 (2008)
	A catalog of bright star clusters in the interacting galaxy M51.
o	Table 1: <[HL2008] NNNNNN> N=2224 among (Nos 459-117066).
=E=	Catalogue in electronic form as <J/AJ/135/1567/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HL2013]
[HL2013]	(Hsieh+Lai, 2013)
Write:	<<[HL2013] DDD.ddddd+DD.ddddd>>
N:	1313
Object:	Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=1313 YSO candidates in 5 star-forming regions using the photometry data from Spitzer's c2d Legacy Project. Use of Spitzer's SWIRE data.
Ref:	=2013ApJS..205....5H
by	HSIEH T.-H. , LAI S.-P.
	Astrophys. J., Suppl. Ser., 205, 5 (2013)
	Populations of young stellar objects in nearby molecular clouds.
o	Table 2: <[HL2013] DDD.ddddd+DD.ddddd> N=1313.
=E=	Catalogue in electronic form as J/ApJS/205/5
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HL85]
[HL85]	(Hartigan+Lada, 1985)= (HL)
Write:	<<[HL85] GGD NN NN>> <<[HL85] GGD NN A>> <<[HL85] GGD NN a>> <<[HL85] GGD NN-NN NN>> <<[HL85] HH NNN NN>> <<[HL85] R CrA a>> <<[HL85] NGC 7129-W R>> <<[HL85] NGC 7129-W NN>>
N:	167
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Stars in the field of HH objects. In the field GGD 37, GGD 29, GGD 1, 31, 36: formats 'GGD NN NN' for * and Rfn or 'GGD NN A' for em. neb. In the field GGD 33, 27, 28: format 'GGD NN a'. In the field GGD 27-28: format 'GGD 27-28 NN'. In the field HH 101, HH 100: format 'HH NNN NN'. In the field R CrA: format 'R CrA a', same objects (Nos a,b, d-h) in [GP75]. In the field NGC 7129-S (South): formats 'NGC 7129-S NN' and 'NGC 7129-S R' In the field NGC 7129-N (North): format 'NGC 7129-N NN', N=18 * among (Nos 1-51)
Ref:	=1985ApJS...59..383H
by	HARTIGAN P. , LADA C.J.
	Astrophys. J., Suppl. Ser., 59, 383-396 (1985)
	CCD images of suspected Herbig-Haro objects.
o	[HL85] RCrA a, b, d to h are identical to [GP75]
o	<HH NNN> (No. 105). Table 2, and text: <[HL85] GGD NN NN>, <[HL85] GGD NN A>, <[HL85] GGD NN a>, <[HL85] GGD NN-NN NN>, <[HL85] HH NNN NN>, <[HL85] RCrA a>, <[HL85] NGC 7129-W R>, <[HL85] NGC 7129-W NN>, N=154.
Ref:	=1990ApJ...360..215H
by	HUGHES V.A. , MORIARTY-SCHIEVEN G.
	Astrophys. J., 360, 215-220 (1990)
	A comparison of the radio continuum and optical properties of the HH objects in Cepheus A West (GGD 37).
o	HW = NAME HW object
o	Table 1: <[HM90] AN> (Nos C1-C3). p.216: <[HL85] GGD 37 A> (No. X) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HL88
HL88	(Hodge+Lee, 1988)
*****	Avoid the usage of HL88, prefer [HLM88]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HL88]
[HL88]	(Heaton+Little, 1988)
Write:	<<[HL88] G35.2N WN>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio components of the radio-source [DLW84] G35.2N.
in source:	GAL 035.2-00.74
Ref:	=1988A&A...195..193H
by	HEATON B.D. , LITTLE L.T.
	Astron. Astrophys., 195, 193-197 (1988)
	Twin beams from a young B star ?
o	Table 1: <[HL88] G35.2N WN> (Nos N, C, S, C2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HL90]
[HL90]	(Hodge+Lee, 1990)= (HL)
Write:	<<[HL90] NNNa>>
N:	157
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Table 2: 153 HII regions (Nos 1-144) with format 'NNNa'
in source:	IC 10
Ref:	=1990PASP..102...26H
by	HODGE P. , LEE M.G.
	Publ. Astron. Soc. Pac., 102, 26-40 (1990)
	The HII regions of IC 10.
o	Table 1: N=9 regions, format A, not in Simbad.
o	Table 2: <[HL90] NNNa> N=157
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HL93]
[HL93]	(Hilton+Lahulla, 1993)
Write:	<<[HL93] NN>>
N:	82
Object:	* (SIMBAD class: Star)
Note:	Tables 1, 2 and 3
in source:	LDN 379
Ref:	=1993AJ....106..672H
by	HILTON J. , LAHULLA J.F.
	Astron. J., 106, 672-675 (1993)
	The distance and structure of L379.
o	Tables 1, 2, 3: <[HL93] NN> N=82
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HL94]
[HL94]	(Heydari-Malayeri+Lecavelier des Etangs, 1994)
Write:	<<[HL94] N4A-N>>
N:	2
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Observations of the HII region LHA 120-N 4A in the LMC: N4A-1 is the brightest component, N4A-2 is a diffuse nebulosity.
in source:	Magellanic Clouds:LMC:LHA 120-N 4A = LHA 120-N 4A
Ref:	=1994A&A...291..960H
by	HEYDARI-MALAYERI M. , LECAVELIER DES ETANGS A.
	Astron. Astrophys., 291, 960-974 (1994)
	The LMC HII region N4A and its unusual molecular cloud.
o	Fig.1: <[HL94] N4A-1>, <[HL94] N4A-2>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HL95]
[HL95]	(Hodapp+Ladd, 1995)= (HL)
Write:	<<[HL95] NGC 1333 IRAS 2 NN>> <<[HL95] LDN 1551 N>> <<[HL95] LDN 1634 NN>> <<[HL95] IRAS 08076-3556 N>>
N:	12+6+11+8
Object:	Knot (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
in source:	NGC 1333:[JCC87] IRAS 2 = [JCC87] IRAS 2
in source:	LDN 1551
in source:	LDN 1634
in source:	IRAS 08076-3556
Ref:	=1995ApJ...453..715H
by	HODAPP K.-W. , LADD E.F.
	Astrophys. J., 453, 715-720 (1995)
	Bipolar jets from extremely young stars observed in molecular hydrogen emission.
o	IRS 3 and 4 in CG 30 = [P84] CG 30 IRS 3 and 4
o	Fig.1: <[HL95] NGC 1333 IRAS 2 NN> (Nos 1-12). Fig.2: <[HL95] LDN 1551 N> (Nos 1-6). Fig.3: <[HL95] LDN 1634 NN> (Nos 1-11). Fig.4: <[HL95] IRAS 08076-3556 N> (Nos 1-8)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLA2019]
[HLA2019]	(Hosek+Lu+Anderson+, 2019)= ([HLA2019a]) (Not yet in Simbad)
Write:	<<[HLA2019] AwNNN NNN>> <<[HLA2019] AwNNN_NNN>> (not recognised by Simbad, but found in literature)
N:	981
Object:	* (SIMBAD class: Star)
Note:	HST WFC3 photometry and Keck I OSIRIS spectroscopy of N=980 stars in the Arches cluster.
Notes:	Naming convention: The first letter is always “A”, followed by "n/s/e/w" to designate whether the star is to the north, south, east or west quadrant relative to the central reference star, as determined using 45° and -45° line boundaries that intersect at the reference star position. The number immediately following gives the radius of the given star relative to the reference in arcseconds, while the second number is a unique index for the star relative to all others at that same radius.
in source:	NAME Arches Cluster
Ref:	=2019ApJ...870...44H
by	HOSEK M.W. , LU J.R., ANDERSON J., NAJARRO F., GHEZ A.M., MORRIS M.R., CLARKSON W.I., ALBERS S.M.
	Astrophys. J., 870, 44-44 (2019)
	The unusual initial mass function of the Arches Cluster.
o	Table 6: <[HLA2019] AwNNN NNN> N=980.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLA2019a]
[HLA2019a]	(Hosek+Lu+Anderson+, 2019) (Not yet in Simbad)
Note:	HST WFC3 photometry and Keck I OSIRIS spectroscopy of N=980 stars
Notes:	Naming convention: The first letter is always “A”, followed by
*****	Avoid the usage of [HLA2019a], prefer [HLA2019]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLA2019b]
[HLA2019b]	(Hernandez+Larsen+Aloisi+, 2019)
Write:	<<[HLA2019b] M83-NN>>
N:	16
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	N=16 young massive stellar clusters in M83. Use of archival HST COS spectroscopic data.
in source:	NGC 5236 = M 83
Ref:	=2019ApJ...872..116H
by	HERNANDEZ S. , LARSEN S., ALOISI A., BERG D.A., BLAIR W.P., FOX A.J., HECKMAN T.M., JAMES B.L., LONG K.S., SKILLMAN E.D., WHITMORE B.C.
	Astrophys. J., 872, 116-116 (2019)
	The first metallicity study of M83 using the integrated UV light of star clusters.
o	Fig. 1, Tables 2-5: <[HLA2019b] M83-NN> (Nos 1-16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLB98]
[HLB98]	(Harju+Lehtinen+Booth+ 1998)
Write:	<<[HLB98] SEST NNN>> <<[HLB98] Onsala NNN>>
N:	184+188
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	SiO emission of interstellar masers using the SEST and Onsala telescopes.
Ref:	=1998A&AS..132..211H
by	HARJU J. , LEHTINEN K., BOOTH R.S., ZINCHENKO I.
	Astron. Astrophys., Suppl. Ser., 132, 211-231 (1998)
	A survey of SiO emission towards interstellar masers. I. SiO line characteristics.
o	Table B1, col(1): <[HLB98] SEST NNN> (Nos 1-184). Table B2, col(1): <[HLB98] Onsala NNN> (Nos 1-188).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLD2018]
[HLD2018]	(Hsu+Lin+Dickinson+, 2018) (Not yet in Simbad)
Write:	<<[HLD2018] NNNNN>>
N:	93598
Object:	(NIR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	CFHT WIRCam observations of N=93598 sources in the extended GOODS North field. Use of archival GALEX, Subaru, Spitzer IRAC, and Chandra data.
in source:	NAME GOODS North Field
Ref:	=2019ApJ...871..233H
by	HSU L.-T. , LIN L., DICKINSON M., YAN H., BAU-CHING H., WANG W.-H., LEE C.-H., YAN C.-H., SCOTT D., WILLNER S.P., OUCHI M., ASHBY M.L.N., CHEN Y.-W., DADDI E., ELBAZ D., FAZIO G.G., FOUCAUD S., HUANG J., KOO D.C., MORRISON G., OWEN F., PANNELLA M., POPE A., SIMARD L., WANG S.-Y.
	Astrophys. J., 871, 233-233 (2019)
	Near-infrared survey and photometric redshifts in the extended GOODS-North field.
o	<[HLD2018] NNNNN> (Nos 1-93598).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HLF
HLF	(High Latitude Field)
Write:	<<HLF 2 SNN>> <<HLF 2 DD NNN>>
N:	1895
Object:	* (SIMBAD class: Star)
Note:	Catalogue of stars in the field HLF 2. Table 3: format '2 SNN' for standard stars (Nos S1-S84) format '2 DD NNN' for stars in declination zones from 11deg to 20deg
Ref:	=1966ApJS...12..391P
by	PHILIP A.G.D.
	Astrophys. J., Suppl. Ser., 12, 391-447 (1966)
	The stellar space distribution in Pegasus at b=-29.
o	Table 1: <HLF Na> (Nos 1-2, 2a, 2b). Table 3: <HLF 2 SNN> (Nos S1-S84), <HLF 2 DD NNN> N=1811
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HLG
HLG	(Hodge+Lee+Gurwell)
*****	Avoid the usage of HLG, prefer [HLG90]
Origin	of the Acronym: L (2001A&A...366...35V)
Details on Acronym: [HLG90]
[HLG90]	(Hodge+Lee+Gurwell, 1990)= (HLG)
Write:	<<[HLG90] NNa>>
N:	100
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Map in Fig.2 See also [S71b] and [VRG2001].
in source:	IC 1613
Ref:	=1990PASP..102.1245H
by	HODGE P. , LEE M.G., GURWELL M.
	Publ. Astron. Soc. Pac., 102, 1245-1262 (1990)
	The H II regions of IC 1613.
o	Table 3: exciting stars [SK76] and [F88b] (which field?) not in SIMBAD.
o	Table 2: <[HLG90] NNa> (Nos 1-77), N=100.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLJ89]
[HLJ89]	(Hammer+Le Fevre+Jones+, 1989)
Write:	<<[HLJ89] A>> <<[HLJ89] A'>> <<[HLJ89] Arc>> <<[HLJ89] Clump A>> <<[HLJ89] Patch N>>
N:	21+1+2+6
Object:	G + Arc (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	Table 1: (Nos A-T, C') are G or lensed images in the field of ClG 2244-02 N=1 Arc. N=2 Clumps (Nos A-B). N=6 Patches, (Nos 1-6).
in source:	ClG 2244-02
Ref:	=1989A&A...208L...7H
by	HAMMER F. , LE FEVRE O., JONES J., RIGAUT F., SOUCAIL G.
	Astron. Astrophys., 208, 7-10 (1989)
	Probable additional gravitational images related to the Cl 2244-02 arc and B, V, R photometry of the cluster core.
o	Table 1: <[HLJ89] A> (Nos A-T), <[HLJ89] C'> N=1, <[HLJ89] Arc> N=1, <[HLJ89] Clump A> (Nos A-B), <[HLJ89] Patch N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLK2010]
[HLK2010]	(Henning+Linz+Krause+, 2010)
Write:	<<[HLK2010] NN>>
N:	24
Object:	Protostar (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	Herschel PACS observations of N=24 protostars in the filamentary IRDC [CCE98b] 011.11-0.12.
in source:	[CCE98b] 011.11-0.12
Ref:	=2010A&A...518L..95H
by	HENNING T. , LINZ H., KRAUSE O., RAGAN S., BEUTHER H., LAUNHARDT R., NIELBOCK M., VASYUNINA T.
	Astron. Astrophys., 518L, 95-95 (2010)
	The seeds of star formation in the filamentary infrared-dark cloud G011.11-0.12.
o	Table 1: <[HLK2010] NN> (Nos 1-24).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLK2018]
[HLK2018]	(Hollyhead+Lardo+Kacharov+, 2018)
Write:	<<[HLK2018] NNNN>>
N:	35
Object:	* (SIMBAD class: Star)
Note:	VLT FORS2 spectroscopic observations of N=35 stars in the SMC stellar cluster Cl Kron 3. See also [HKL2017].
in source:	Cl Kron 3
Ref:	=2018MNRAS.476..114H
by	HOLLYHEAD K. , LARDO C., KACHAROV N., BASTIAN N., HILKER M., REJKUBA M., KOCH A., GREBEL E.K., GEORGIEV I.
	Mon. Not. R. Astron. Soc., 476, 114-121 (2018)
	Kron 3: a fourth intermediate age cluster in the SMC with evidence of multiple populations.
o	Table 1: <[HLK2018] NNNN> N=35 among (Nos 129-7963).
=E=	Catalogue in electronic form as <J/MNRAS/476/114/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLK89]
[HLK89]	(Hodge+Lee+Kennicutt, 1989)= (HL)
Write:	<<[HLK89] NNa>>
N:	22
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-22), (Nos 5a-5e), and (Nos 19a-19f)
in source:	GRDG 8
Ref:	=1989PASP..101..640H
by	HODGE P. , LEE M.G., KENNICUTT R.C.
	Publ. Astron. Soc. Pac., 101, 640-648 (1989)
	The HII regions of GR8.
o	<[HLK89] NNa> N=33
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HLL2005]
[HLL2005]	(Hwang+Lee+Lee+, 2005)
Write:	<<[HLL2005] SCN>>
N:	3
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	CFHT MegaPrime observations. Discovery of N=3 new star clusters in NGC 6822.
in source:	NGC 6822
Ref:	=2005IAUCo.198..257H
by	HWANG N. , LEE M.G., LEE J.C., PARK W.-K., PARK H.S., PARK J.-H., SOHN S.T., LEE S.-G., LEE H.M., CHUN M.-S., LEE Y.-W., SOHN Y.-J., YUK I.-S., KIM S.C., KIM H.-I., HAN W.
	IAUCo, 198, 257-258 (2005)
	Discovery of remote star clusters in the halo of the irregular galaxy NGC 6822.
o	Fig.1: <[HLL2005] SCN> (Nos SC1-SC3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLL2007]
[HLL2007]	(Hwang+Lee+Lee+, 2007)
Write:	<<[HLL2007] NNNNNN>>
N:	about 56000
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	CFHT Megacam photometric catalog of sources in the NEP.
in source:	NAME NEP
Ref:	=2007ApJS..172..583H
by	HWANG N. , LEE M.G., LEE H.M., IM M., KIM T., MATSUHARA H., WADA T., OYABU S., PAK S., CHUN M.-Y., WATARAI H., NAKAGAWA T., PEARSON C., TAKAGI T., HANAMI H., WHITE G.J.
	Astrophys. J., Suppl. Ser., 172, 583-598 (2007)
	An optical source catalog of the North Ecliptic Pole region.
o	Table 2: <[HLL2007] NNNNNN> N=about 56000 among (Nos 3-116549).
=E=	Catalogue in electronic form as J/ApJS/172/583
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLL2011]
[HLL2011]	(Hwang+Lee+Lee+, 2011)
Write:	<<[HLL2011] NGC 6822CN>>
N:	4
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	CFHT MegaCam observations of N=4 star clusters in NGC 6822.
in source:	NGC 6822
Ref:	=2011ApJ...738...58H
by	HWANG N. , LEE M.G., LEE J.C., PARK W.-K., PARK H.S., KIM S.C., PARK J.-H.
	Astrophys. J., 738, 58 (2011)
	Extended star clusters in the remote halo of the intriguing dwarf galaxy NGC 6822.
o	Figs 1-2, Table 1: <[HLL2011] NGC6822CN> (Nos C1-C4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLL2020]
[HLL2020]	(Hui+Lee+Li+, 2020)
Write:	<<[HLL2020] JHHMMm XN>> <<[HLL2020] JHHMMm_XN>> (not recognised by Simbad, but found in literature)
N:	36
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	N=36 X-ray sources in the field of ten 3FHL pulsar-like candidates. Use of archival Chandra, XMM-Newton, Swift data.
Ref:	=2020MNRAS.495.1093H
by	HUI C.Y. , LEE J., LI K.L., KIM S., OH K., LUO S., LEUNG A.P., KONG A.K.H., TAKATA J., CHENG K.S.
	Mon. Not. R. Astron. Soc., 495, 1093-1109 (2020)
	Searches for pulsar-like candidates from unidentified objects in the Third Catalog of Hard Fermi-LAT Sources with machine learning techniques.
o	Fig. 4, Table 4: <[HLL2020] JHHMMm XN> N=36.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLL97]
[HLL97]	(Horner+Lada+Lada, 1997)
Write:	<<[HLL97] NNN>> <<[HLL97] A>>
N:	394+4
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Table 3: (Nos 1-394) IR in a young cluster associated with NGC 2282 Fig.1: (Nos A-D), 4 nebulous IR sources.
in source:	NGC 2282
Ref:	=1997AJ....113.1788H
by	HORNER D.J. , LADA E.A., LADA C.J.
	Astron. J., 113, 1788-1798 (1997)
	A near-infrared imaging survey of NGC 2282.
o	Table 3: <[HLL97] NNN> N=394. Fig.1: <[HLL97] A> (Nos A-D)
=E=	Catalogue in electronic form as J/AJ/113/1788
Details on Acronym: [HLM2019]
[HLM2019]	(Hankins+Lau+Mills+, 2019) (Not yet in Simbad)
Write:	<<[HLM2019] Sgr A-HNWW>> <<[HLM2019] Sgr A-H3NN>>
N:	7
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	SOFIA/FORCAST IR observations of N=7 sub-regions within the Sgr A-H H II regions. Use of archival HST, 2MASS and Spitzer IRAC data.
in source:	[HJB85] Sgr A-H
Ref:	=2019ApJ...877...22H
by	HANKINS M.J. , LAU R.M., MILLS E.A.C., MORRIS M.R., HERTER T.L.
	Astrophys. J., 877, 22-22 (2019)
	SOFIA/FORCAST observations of the Sgr A-H H II regions: using dust emission to elucidate the heating sources.
o	Tables 2/5: <[HJB85] Sgr A-HNN> (Nos H14-H21) added. Table 5: <[HJB85] Sgr A-HNNa> (Nos H22c, H23c) added. Table 4: <[HLM2019] Sgr A-HNWW> (Nos H2NE, H2SW, H3S, H5E and H5W) N=5, <[HLM2019] Sgr A-H3NN> (Nos H3N1, H3N2) N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLM88]
[HLM88]	(Hodge+Lee+Mateo, 1988)= (HL88)
Write:	<<[HLM88] ANNN>>
N:	695+122+220+224+226+341
Object:	* (SIMBAD class: Star)
Note:	ref. 1988ApJ...324..172H: * in the 1st field, named field 'A' in the 2nd ref. ref. 1988ApJ...329..651H: * in the fields 'C, D, E, I, J'
in source:	M 31 = NGC 224
Ref:	=1988ApJ...324..172H
by	HODGE P. , LEE M.G., MATEO M.
	Astrophys. J., 324, 172-192 (1988)
	UBVR CCD photometry of stars in M 31. I. Baade's field IV.
o	Table 1: the field is named field 'A' in the 2nd ref 1988ApJ.329.651H. Tables 2-5: obj. are '[BS63]'
o	Table 1: <[HLM88] ANNN> (Nos 1-695)
Ref:	=1988ApJ...329..651H
by	HODGE P. , LEE M.G.
	Astrophys. J., 329, 651-686 (1988)
	UBVR CCD photometry of stars in M 31. II. Five disk fields.
o	see also paper I: 1988ApJ...324..172H
o	Tables 2A-2E: <[HLM88] CNNN> (Nos 1-122), <[HLM88] DNNN> (Nos 1-220), <[HLM88] ENNN> (Nos 1-224), <[HLM88] INNN> (Nos 1-226), <[HLM88] JNNN> (Nos 1-341)
=E=	Catalogue in electronic form as J/ApJ/324/172
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Hln
Hln	(Holden)
Write:	<<** HLN NN>>
N:	17
Object:	(SIMBAD class: = Double or Multiple Star)
Ref:	=1974PASP...86..907H
by	HOLDEN F.
	Publ. Astron. Soc. Pac., 86, 907-911 (1974)
	Measures of southern visual double stars.
o	RST 5201 misprint for RST 5021
o	<** Hln NN> (Nos 1-17)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HLR2013]
[HLR2013]	(Huang+Li+Rector+, 2013)
Write:	<<[HLR2013] NN>>
N:	16
Object:	YSO + Be* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	NAOC 2.16m telescope and KPNO Mayall 4m telescope observations of N=15 YSOs and N=1 Be star toward IC 1396. Use of 2MASS and AKARI data.
Ref:	=2013AJ....145..126H
by	HUANG Y.F. , LI J.Z., RECTOR T.A., MALLAMACI C.C.
	Astron. J., 145, 126 (2013)
	Efficient selection and classification of infrared excess emission stars based on AKARI and 2MASS data.
o	Table 3: <[HLR2013] NN> (Nos 1-16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLR76]
[HLR76]	(Harper+Low+Rieke+, 1976)
Write:	<<[HLR76] IRe Na>> <<[HLR76] IRc N>>
N:	8+2
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Infrared emission from M 17: compact (IRc) and extended (IRe) sources are found.
in source:	M 17 = NGC 6618
Ref:	=1976ApJ...205..136H
by	HARPER D.A. , LOW F.J., RIEKE G.H., HARLEY A., THRONSON H.A.Jr
	Astrophys. J., 205, 136-143 (1976)
	The infrared emission of M 17.
o	Table 1: <[HLR76] IRe Na> (Nos 1, 2a-2c, 3-6), <[HLR76] IRc N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HLS
HLS	(Herschel Lensing Survey)
*****	Avoid the usage of HLS, prefer [CRR2012]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HLS
HLS	(Hoffman+Lu+Salpeter)
Write:	<<HLS GNN>>
N:	11
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	The format 'GNN' (G for Galaxy) is used by the authors, the format 'NN' is found in the literature. No identif. charts.
Ref:	=1992AJ....104.2086H
by	HOFFMAN G.L. , LU N.Y., SALPETER E.E.
	Astron. J., 104, 2086-2096 (1992)
	A search for gas-rich dwarf galaxies just outside the local supercluster.
o	<HLS GNN> (Nos G1-G11).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HLS
HLS	(Herschel Lensing Survey)
*****	Avoid the usage of HLS, prefer [RRE2010]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HLS
HLS	(Herschel Lensing Survey)
*****	Avoid the usage of HLS, prefer [RRE2012]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HLS
HLS	(Herschel Lensing Survey)
*****	Avoid the usage of HLS, prefer [ZYA2015]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HLS2000]
[HLS2000]	(Henning+Lapinov+Schreyer+, 2000)= (MIR)
Write:	<<[HLS2000] MIR N>>
N:	4
Object:	(Mid IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Mid-infrared image of IRAS 12326-6245.
in source:	IRAS 12326-6245
Ref:	=2000A&A...364..613H
by	HENNING T. , LAPINOV A., SCHREYER K., STECKLUM B., ZINCHENKO I.
	Astron. Astrophys., 364, 613-624 (2000)
	IRAS 12326-6245: Luminous very young stellar objects with a massive molecular outflow.
o	Fig.2, Table 4: <[HLS2000] MIR N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLS2010]
[HLS2010]	(Hilton+Lloyd-Davies+Stanford+, 2010)
Write:	<<[HLS2010] PSN>> <<[HLS2010] NNN>>
N:	3+44
Object:	(X) + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Chandra ACIS observations of N=3 point sources and Keck II DEIMOS and GMOS observations of N=44 galaxies in the cluster XMMXCS J2215.9-1738.
in source:	XMMXCS J2215.0-1738
Ref:	=2010ApJ...718..133H
by	HILTON M. , LLOYD-DAVIES E., STANFORD S.A., STOTT J.P., COLLINS C.A., ROMER A.K., HOSMER M., HOYLE B., KAY S.T., LIDDLE A.R., MEHRTENS N., MILLER C.J., SAHLEN M., VIANA P.T.P.
	Astrophys. J., 718, 133-147 (2010)
	The XMM cluster survey: active galactic nuclei and starburst galaxies in XMMXCS J2215.9-1738 at z = 1.46.
o	In table 2, [HSS2009b] 859 is a misprint for [HSS2009b] 858.
o	Fig. 1, Table 1: <[HLS2010] PSN> (Nos PS1-PS3). Table 2: <[HLS2010] NNN> N=44 among (Nos 1-883).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLS2016]
[HLS2016]	(Huang+Lemaux+Schmidt+, 2016)
Write:	<<[HLS2016] MACS J2129 source>> <<[HLS2016] MACS J2129 A>>
N:	1+3
Object:	G + Grav. lensed image of a G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Keck DEIMOS observations of N=3 gravitationally lensed images of N=1 galaxy at z=6.85, lensed by the galaxy cluster MCS J2129.4-0741. Use of HST Grism Lens-Amplified Survey from Space (GLASS) data. Use of Cluster Lensing And Supernova survey with Hubble (CLASH) and Spitzer IRAC data.
in source:	ClG J2129-0741 = MCS J2129.4-0741
Ref:	=2016ApJ...823L..14H
by	HUANG K.-H. , LEMAUX B.C., SCHMIDT K.B., HOAG A., BRADAC M., TREU T., DIJKSTRA M., FONTANA A., HENRY A., MALKAN M., MASON C., MORISHITA T., PENTERICCI L., RYAN R.E., TRENTI M., WANG X.
	Astrophys. J., 823L, 14-14 (2016)
	Detection of Lyman-α emission from a triply imaged z = 6.85 galaxy behind MACS J2129.4-0741.
o	<[HLS2016] MACS J2129 source> N=1. Fig. 1, Table 1: <[HLS2016] MACS J2129 A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLS2017]
[HLS2017]	(Hughes+Lacy+Sakari+, 2017)
Write:	<<[HLS2017] NNN>>
N:	218
Object:	* (SIMBAD class: Star)
Note:	Apache Point Observatory 3.5m telescope spectroscopic observations of N=218 stars in the field of Segue 3. Use of archival SDSS DR13 data. See also [FWG2011] and [OBB2013].
in source:	NAME Segue 3
Ref:	=2017AJ....154...57H
by	HUGHES J. , LACY B., SAKARI C., WALLERSTEIN G., DAVIS C.E., SCHIEFELBEIN S., CORRIN O., JOUDI H., LE D., HAYNES R.M.
	Astron. J., 154, 57-57 (2017)
	A multiwavelength study of the Segue 3 cluster.
o	Tables 2-3: <[HLS2017] NNN> N=218 among (Nos 2-304).
=E=	Catalogue in electronic form as J/AJ/154/57
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLS99]
[HLS99]	(Hoffman+Lu+Salpeter+, 1999)
Write:	<<[HLS99] Cloud A>>
N:	3
Object:	Cloud (SIMBAD class: Cloud)
Note:	Map in Fig.2: Gaz concentrations outside the galaxies, Cloud A and Cloud B are HI concentrations Cloud A is in DDO 137. Cloud B is within the West extended plume of DDO 137. Cloud C is a HI concentration in NGC 4532.
in source:	DDO 137
in source:	NGC 4532
Ref:	=1999AJ....117..811H
by	HOFFMAN G.L. , LU N.Y., SALPETER E.E., CONNELL B.M.
	Astron. J., 117, 811-825 (1999)
	Dark matter and gas concentrations in the NGC 4532/DDO 137 system.
o	Table 4: <[HLS99] Cloud A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLT99]
[HLT99]	(Hines+Low+Thompson+, 1999)
Write:	<<[HLT99] Ring G>> <<[HLT99] Host G>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Observations of the QSO PG 1700+518, its companion ring galaxy, and its Host galaxy. [HLT99] Ring G = PG 1700+518R
in source:	PG 1700+518
Ref:	=1999ApJ...512..140H
by	HINES D.C. , LOW F.J., THOMPSON R.I., WEYMANN R.J., STORRIE-LOMBARDI L.J.
	Astrophys. J., 512, 140-144 (1999)
	The host galaxy of the broad absorption line QSO PG 1700+518 and its ring galaxy companion: NICMOS 1.6 micron imaging.
o	[HLT99] Ring G = PG 1700+518R
o	<[HLT99] Ring G> N=1, <[HLT99] Host G> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLV92]
[HLV92]	(Hoekzema+Lamers+Van Genderen, 1992)
Write:	<<[HLV92] NNNAA>>
N:	43
Object:	* (SIMBAD class: Star)
Note:	Table 3: N=43 among (Nos 1-193)
Ref:	=1992A&A...257..118H
by	HOEKZEMA N.M. , LAMERS H.J.G.L.M., VAN GENDEREN A.M.
	Astron. Astrophys., 257, 118-127 (1992)
	The distance and reddening of stars near the luminous blue variable AG Carinae.
o	Table 3: <[HLV92] NNNAA> N=43 among 195
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLV93]
[HLV93]	(Hoekzema+Lamers+Van Genderen, 1993)
Write:	<<[HLV93] NNN>> <<[HLV93] NNNbis>> <<[HLV93] NNNbisA>>
N:	114
Object:	* (SIMBAD class: Star)
Note:	N=114 among (Nos 0-199)
Ref:	=1993A&AS...98..505H
by	HOEKZEMA N.M. , LAMERS H.J.G.L.M., VAN GENDEREN A.M.
	Astron. Astrophys., Suppl. Ser., 98, 505-511 (1993)
	Walraven photometry of stars near the luminous blue variable AG Carinae.
o	<[HLV93] NNN>, <[HLV93] NNNbis>, <[HLV93] NNNbisA>, N=114 among (Nos 0-199)
=E=	Catalogue in electronic form as J/A+AS/98/505
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HLW2002]
[HLW2002]	(Hutchings+Li+Wood-Vasey+, 2002)
Write:	<<[HLW2002] JHHMMSS.ss+DDMMSS.s>>
N:	4
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxies of SN 2002EV, SN 2002EW, SN 2002EX, SN 2002EY.
Ref:	=2002IAUC.7964....1H
by	HUTCHINGS D. , LI W.D., WOOD-VASEY W.M., ALDERING G., NUGENT P.
	IAU Circ., 7964, 1-None (2002)
	Supernovae 2002ev, 2002ew, 2002ex, 2002ey.
o	<[HLW2002] JHHMMSS.ss+DDMMSS.s> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HM
HM	(Howard+Maran) (Not yet in Simbad)
*****	Avoid the usage of HM, prefer [HM65]
Details on Acronym: HM
HM	(Hoskins+Murdoch) (Not yet in Simbad)
*****	Avoid the usage of HM, prefer MLO
Details on Acronym: HM
HM	(Henize+Mendoza)
*****	Avoid the usage of HM, prefer Ass Cha T
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HM
HM	(Havlen+Moffat)= (Havlen-Moffat)
Write:	<<Cl HM N>>
N:	1
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Stat:	is completely incorporated in Simbad
Note:	N=1, Cl HM 1 = C 1715-387
Ref:	=1977A&A....58..351H
by	HAVLEN R.J. , MOFFAT A.F.J.
	Astron. Astrophys., 58, 351-356 (1977)
	A new cluster containing 2 Wolf-Rayet stars and 2 Of stars.
o	<Cl HM 1>, Table 1: <Cl HM 1 NN> (Nos 1-24)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HM
HM	(Haro+Moreno)
*****	Avoid the usage of HM, prefer Haro
Details on Acronym: HM
HM	(Heydari-Malayeri+)
*****	Avoid the usage of HM, prefer [HGM93]
Origin	of the Acronym: L (2000AJ....119.2214M)
Details on Acronym: HM
HM	(Herbig+Mendoza)
*****	Avoid the usage of HM, prefer [HM60]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HM
HM	(Hodge+Miller)
*****	Avoid the usage of HM, prefer [HM95]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HM2001]
[HM2001]	(Harutyunian+Melikian, 2001)
Write:	<<[HM2001] N>>
N:	3
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
in source:	NAME Cyg Region
Ref:	=2001Ap.....44..352H
by	HARUTYUNIAN H.A. , MELIKIAN N.D.
	Astrophysics, 44, 352-358 (2001)
	Brightness variation and proper motions of three objects in the Cygnus region.
o	Table 1: <[HM2001] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HM2002]
[HM2002]	(Holovatyy+Melekh, 2002) (Not yet in Simbad)
Write:	<<[HM2002] NN>> <<[HM2002] HHMM+DDd>> <<[HM2002] HHMM+DDdA>> <<[HM2002] HHMM+DDdW>> <<[HM2002] I Zw 18 WW>>
N:	41
Object:	HII (SIMBAD class: HIIReg = HII Region)
Ref:	=2002ARep...46..779H
by	HOLOVATYI V.V. , MELEKH B.Y.
	Astron. Rep., 46, 779-790 (2002)
	The chemical composition of HII regions in blue compact dwarf galaxies.
o	2002AZh....79..867H
o	Table 2: <[HM2002] NN> (Nos 1-41) = <[HM2002] HHMM+DDd>, <[HM2002] HHMM+DDdA>, <[HM2002] HHMM+DDdW>, <[HM2002] I Zw 18 WW>, N=41.
=E=	Catalogue in electronic form as J/AZh/79/867
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HM2006]
[HM2006]	(Holland+Marshall, 2006)
Write:	<<[HM2006] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Swift UVOT observations of GRB 061201.
Ref:	=2006GCN..5883....1H
by	HOLLAND S.T. , MARSHALL F.
	GCN, 5883, 1 (2006)
	GRB 061201: initial UVOT observations.
o	<[HM2006] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HM2015]
[HM2015]	(Hoffmann+Macri, 2015)= ([HM2015a])
Write:	<<[HM2015] CNNN>> <<[HM2015] VNNN>>
N:	94+215
Object:	Cepheid + V* (SIMBAD class: Variable* = Variable Star)
Note:	Gemini North GMOS and WIYN MiniMosaic observations of N=94 Cepheid and N=215 variable stars in NGC 4258.
in source:	NGC 4258
Ref:	=2015AJ....149..183H
by	HOFFMANN S.L. , MACRI L.M.
	Astron. J., 149, 183 (2015)
	Cepheid variables in the maser-host galaxy NGC 4258.
o	Fig. 6, Table 6: <[HM2015] CNNN> (Nos C001-C094). Fig. 6, Table 7: <[HM2015] VNNN> (Nos V001-V215).
=E=	Catalogue in electronic form as J/AJ/149/183
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HM2015a]
[HM2015a]	(Hoffmann+Macri, 2015)
*****	Avoid the usage of [HM2015a], prefer [HM2015]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HM2015b]
[HM2015b]	(Hernandez-Fernandez+Mendes De Oliveira, 2015)
Write:	<<[HM2015b] NNN>> <<[HM2015b] NNN N>>
N:	280+1193
Object:	Group of G + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Catalog of N=280 star-forming compact groups (SFCGs) of galaxies in the Local Universe at z<0.15 and a catalog of N=1193 UV-bright group member galaxies. Use of GALEX All-sky Imaging Survey.
Ref:	=2015MNRAS.453.1965H
by	HERNANDEZ-FERNANDEZ J.D. , MENDES DE OLIVEIRA C.
	Mon. Not. R. Astron. Soc., 453, 1965-1980 (2015)
	Star-forming compact groups (SFCGs): an ultraviolet search for a local sample.
o	Table 1: <[HM2015b] NNN> (Nos 1-280). Table 2: <[HM2015b] NNN N> N=1193 among (Nos 1 4 to 280 7).
=E=	Catalogue in electronic form as J/MNRAS/453/1965
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HM60]
[HM60]	(Herbig+Mendoza, 1960)= (HM)
Write:	<<[HM60] N>>
N:	3
Object:	WR* (SIMBAD class: WolfRayet* = Wolf-Rayet)
Stat:	is completely incorporated in Simbad
Ref:	=1960BOTT....2s..21H
by	HERBIG G.H. , MENDOZA E.E.
	Bol. Obs. Tonantz. Tacub., 2, part no 19, 21-23 (1960)
	Wolf-Rayet stars in the vicinity of the association VI Cygni.
o	<[HM60] N> (Nos 1-3)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HM65]
[HM65]	(Howard+Maran, 1965)= (HM) (Not yet in Simbad)
Write:	<<[HM65] NNNN>>
N:	1293
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1965ApJS...10....1H
by	HOWARD III W.E. , MARAN S.P.
	Astrophys. J., Suppl. Ser., 10, 1-330 (1965)
	General catalogue of discrete radio sources.
o	Tables 1, 2: <[HM65] NNNN> (Nos 1-1293)
Details on Acronym: [HM82]
[HM82]	(Hoessel+Mould, 1982)
Write:	<<[HM82] NNN>> <<[HM82] AN>>
N:	388+3
Object:	* + Cluster of * (SIMBAD class: Star)
Note:	Palomar observations of the Pegasus dwarf irregular galaxy. See also: [HSD83], [HD83], [HD84], [HA86]
in source:	NAME Peg Galaxy
Ref:	=1982ApJ...254...38H
by	HOESSEL J.G. , MOULD J.R.
	Astrophys. J., 254, 38-49 (1982)
	Photometry of resolved galaxies. I. The Pegasus dwarf irregular.
o	Table 1: objects are not in SIMBAD
o	Table 1: <[HM82] NNN> (Nos 100-487). Table 2: [HM82] AN> (Nos A1-A3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HM85]
[HM85]	(Hopp+Materne, 1985)
Write:	<<[HM85] NN>>
N:	34
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	Str 0625-540
in source:	Str 0627-544
Ref:	=1985A&A...148..359H
by	HOPP U. , MATERNE J.
	Astron. Astrophys., 148, 359-363 (1985)
	Observations of the southern galaxy clusters STR 0625-540 and STR 0627-544.
o	Table 1: <[HM85] NN> (Nos 1-34).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HM89]
[HM89]	(Hamuy+Maza, 1989)
Write:	<<[HM89] Ton S 180 N>> <<[HM89] Frl NN N>> <<[HM89] NGC NNNN NN>> <<[HM89] PKS HHMM+DDd N>> <<[HM89] MCG -5-23-16 N>> <<[HM89] IC 4329A NN>>
N:	84
Object:	* (SIMBAD class: Star)
Note:	N=84 stars in the fields of 12 active galaxies. Finding charts.
Ref:	=1989AJ.....97..720H
by	HAMUY M. , MAZA J.
	Astron. J., 97, 720-725 (1989)
	UBVRI photoelectric photometry in the fields of fifteen active galaxies.
o	Star 'A' in the field of 3C 273 = [S65] A
o	Table II: <[HM89] Ton S 180 N>, <[HM89] Frl NN N>, <[HM89] NGC NNNN NN>, <[HM89] PKS HHMM+DDd N>, <[HM89] MCG -5-23-16 N>, <[HM89] IC 4329A NN>, N=84. <[M81b] Akn 120 A> (Nos J-N) added. <[M81b] Mrk 509 A> (Nos G-I) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HM90]
[HM90]	(Hughes+Moriarty-Schieven, 1990)= ([GRR96]) = ([HM90a])
Write:	<<[HM90] CN>>
N:	4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	In the format, the letter 'C' stands for Control source
in source:	GGD 37
Ref:	=1990ApJ...360..215H
by	HUGHES V.A. , MORIARTY-SCHIEVEN G.
	Astrophys. J., 360, 215-220 (1990)
	A comparison of the radio continuum and optical properties of the HH objects in Cepheus A West (GGD 37).
o	HW = NAME HW object
o	Table 1: <[HM90] AN> (Nos C1-C3). p.216: <[HL85] GGD 37 A> (No. X) added.
Ref:	=1996ApJ...459..193G
by	GARAY G. , RAMIREZ S., RODRIGUEZ L.F., CURIEL S., TORRELLES J.M.
	Astrophys. J., 459, 193-208 (1996)
	The nature of the radio sources within the Cepheus A star-forming region.
o	Table 5: <[HM90] CN> (No. 4) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HM90a]
[HM90a]	(Hughes+Moriarty-Schieven, 1990)
*****	Avoid the usage of [HM90a], prefer [HM90]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HM90b]
[HM90b]	(Hunter+Massey, 1990)
Write:	<<[HM90b] SNNN N>>
N:	64
Object:	* (SIMBAD class: Star)
Note:	KPNO 2.1m telescope spectroscopic observations of N=64 stars in the field of 36 HII regions. See also [CGG78], [F89b], [L85].
Ref:	=1990AJ.....99..846H
by	HUNTER D.A. , MASSEY P.
	Astron. J., 99, 846-856 (1990)
	Small galactic HII regions. I. Spectral classifications of massive stars.
o	Table I: <[HM90b] SNNN N> N=64.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HM95]
[HM95]	(Hodge+Miller, 1995)= (HM)
Write:	<<[HM95] WLM NNWW>> <<[HM95] WLM NNa>> <<[HM95] EGB 0427+63 NN>> <<[HM95] UGCA 86 NNN>>
N:	21+4+25+115
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Table 2: HII regions in dwarf galaxies. In WLM: format 'WLM NN', (Nos 1-21), No. 16 is later separate in two regions NW and SE, and two compact regions are added east of No. 18 and designated 18a and 18b. In EGB 0427+63: format 'EGB 0427+63 NN', (Nos 1-25) In UGCA 86: format 'UGC-A 86 NNN', (Nos 1-115)'
in source:	DDO 221 = WLM Galaxy
in source:	EGB 0427+63
in source:	UGCA 86
Ref:	=1995ApJ...451..176H
by	HODGE P. , MILLER B.W.
	Astrophys. J., 451, 176-187 (1995)
	H II regions in four galaxies in and near the Local Group.
o	Fig.1: Complexes C1 and C2 are [HHG93] DDO 221 1 and [HHG93] DDO 221 2.
o	Table 2: <[HM95] WLM NN> (Nos 1-21), <[HM95] EGB 0427+63 NN> (Nos 1-25), <[HM95] UGCA 86 NNN> (Nos 1-115)
Ref:	=2005ApJ...620..223L
by	LEE H. , SKILLMAN E.D., VENN K.A.
	Astrophys. J., 620, 223-237 (2005)
	Investigating the possible anomaly between nebular and stellar oxygen abundances in the dwarf irregular galaxy WLM.
o	Stars WLM 15, 30 and 31 are [SC85b] 15, ...30, ...31
o	Table 3: <[HM95] WLM NNWW> (Nos 16NW, 16SE) added, <[HM95] WLM NNa> (Nos 18a, 18b) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HM98]
[HM98]	(Hickson+Mulrooney, 1998)
Write:	<<[HM98] JHHMM+DD>>
N:	21
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Faint spectrophotometric standards. Format 'JHHMM+DD': rounded 2000.0 coordinates. Finding charts
Ref:	=1998ApJ...506..191H
by	HICKSON P. , MULROONEY M.K.
	Astrophys. J., 506, 191-204 (1998)
	A series of faint spectrophotometric standard stars at +33° declination.
o	Table 1: <[HM98] JHHMM+DD> N=21.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMA2000]
[HMA2000]	(Hernandez+Meikle+Aparicio+, 2000) (Not yet in Simbad)
Write:	<<[HMA2000] CSN>>
N:	5
Object:	* (SIMBAD class: Star)
Note:	N=5 Comparison Stars (CS in the format) in the field of SN 1998BU.
Ref:	=2000MNRAS.319..223H
by	HERNANDEZ M. , MEIKLE W.P.S., APARICIO A., BENN C.R., BURLEIGH M.R., CHRYSOSTOMOU A.C., FERNANDES A.J.L., GEBALLE T.R., HAMMERSLEY P.L., IGLESIAS-PARAMO J., JAMES D.J., JAMES P.A., KEMP S.N., LISTER T.A., MARTINEZ-DELGADO D., OSCOZ A., POLLACCO D.L., ROZAS M., SMARTT S.J., SORENSEN P., SWATERS R.A., TELTING J.H., VACCA W.D., WALTON N.A., ZAPATERO-OSORIO M.R.
	Mon. Not. R. Astron. Soc., 319, 223-234 (2000)
	An early-time infrared and optical study of the Type Ia Supernova 1998bu in M96.
o	Fig.1, Table 1: <[HMA2000] CSN> (Nos CS1-CS5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMA2011]
[HMA2011]	(Habibi+Moniez+Ansari+, 2011)
Write:	<<[HMA2011] 4338>>
N:	1
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	ESO NTT SOFI observations of N=1 star toward the Barnard 68 nebula.
in source:	Barnard 68
Ref:	=2011A&A...525A.108H
by	HABIBI F. , MONIEZ M., ANSARI R., RAHVAR S.
	Astron. Astrophys., 525A, 108-108 (2011)
	Searching for galactic hidden gas through interstellar scintillation: results from a test with the NTT-SOFI detector.
o	Fig. 10, Paragr. 5.4: <[HMA2011] 4338> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMA92a]
[HMA92a]	(Hamuy+Maza+Antezana+, 1992)
Write:	<<[HMA92a] HHMMSS+DDMM.m>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of SN 1992AQ.
Ref:	=1992IAUC.5574....1H
by	HAMUY M. , MAZA J., ANTEZANA R., WELLS L., MUENA C., WILLIAMS R., AVILES R., SMITH R.C.
	IAU Circ., 5574, 1-1 (1992)
	Supernovae 1992aq and 1992ar in anonymous galaxies.
o	<[HMA92a] HHMMSS+DDMM.m> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMA92b]
[HMA92b]	(Hamuy+Maza+Antezana+, 1992)
Write:	<<[HMA92b] HHMMSS+DDMM.m>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of SN 1992AU.
Ref:	=1992IAUC.5584Q...1H
by	HAMUY M. , MAZA J., ANTEZANA R., WISCHNJEWSKY M., AVILES R.
	IAU Circ., 5584, 1-None (1992)
	Supernova 1992au in anonymous galaxy.
o	<[HMA92b] HHMMSS+DDMM.m> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMA93]
[HMA93]	(Hamuy+Maza+Antezana+, 1993)
Write:	<<[HMA93] HHMMSS+DDMM.m>> <<[HMA93] HHMMSS.s+DDMMSS>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxies of SN 1993O and SN 1993P.
Ref:	=1993IAUC.5799....1H
by	HAMUY M. , MAZA J., ANTEZANA R., VALLADARES G., LAYDEN A., PHILLIPS M.M.
	IAU Circ., 5799, 1-None (1993)
	Supernovae 1993O and 1993P in anonymous galaxies.
o	<[HMA93] HHMMSS+DDMM.m> N=1, <[HMA93] HHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMB94]
[HMB94]	(Hook+McMahon +Boyle+, 1994)
Write:	<<[HMB94] HHMMSS.ss+DDMMSS.s>>
N:	332
Object:	QSO (SIMBAD class: QSO = Quasar)
Ref:	=1994MNRAS.268..305H
by	HOOK I.M. , McMAHON R.G., BOYLE B.J., IRWIN M.J.
	Mon. Not. R. Astron. Soc., 268, 305-320 (1994)
	The variability of optically selected quasars.
o	Table A1: <[HMB94] HHMMSS.ss+DDMMSS.s> N=332
=E=	Catalogue in electronic form as J/MNRAS/268/305
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMB97]
[HMB97]	(Haberl+Motch+Buckley+, 1997)
Write:	<<[HMB97] A>>
N:	3
Object:	* (SIMBAD class: Star)
Note:	EXOSAT and ROSAT observations. N=3 faint objects in the field of RX J0720.4-3125. See also [MH98]
Ref:	=1997A&A...326..662H
by	HABERL F. , MOTCH C., BUCKLEY D.A.H., ZICKGRAF F.-J., PIETSCH W.
	Astron. Astrophys., 326, 662-668 (1997)
	RXJ0720.4-3125: strong evidence for an isolated pulsating neutron star.
o	Fig.7: <[HMB97] A> (Nos A-C)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMC2003]
[HMC2003]	(Hutchings+Maddox+Cutri+, 2003)= ([HMC2003a])
Write:	<<[HMC2003] JHHMMSS.ss+DDMMSS.s>>
N:	76
Object:	AGN (SIMBAD class: AGN = Active Galaxy Nucleus)
Stat:	is completely incorporated in Simbad
Note:	Optical imaging of 76 low redshift IR-selected AGNs (2MASS AGNs with z<0.3, observable from CFHT). See also [HCC2006].
Ref:	=2003AJ....126...63H
by	HUTCHINGS J.B. , MADDOX N., CUTRI R.M., NELSON B.O.
	Astron. J., 126, 63-72 (2003)
	Host galaxies of 2MASS-Selected QSOs to redshift 0.3.
o	Table 1: <[HMC2003] JHHMMSS.ss+DDMMSS.s> N=76.
=E=	Catalogue in electronic form as J/AJ/126/63
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMC2003a]
[HMC2003a]	(Hutchings+Maddox+Cutri+, 2003)
*****	Avoid the usage of [HMC2003a], prefer [HMC2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMC2003b]
[HMC2003b]	(Heydari-Malayeri+Meynadier+Chamandaris+, 2003)
Write:	<<[HMC2003b] NNN>>
N:	42
Object:	* (SIMBAD class: Star)
Note:	ISAAC camera at the ESO VLT observations. Table 1: Only brightest stars towards N81 (LHA 115-N 81) are in the table. See also [HRZ99].
Ref:	=2003A&A...411..427H
by	HEYDARI-MALAYERI M. , MEYNADIER F., CHARMANDARIS V., DEHARVENG L., LE BERTRE T., ROSA M.R., SCHAERER D.
	Astron. Astrophys., 411, 427-435 (2003)
	The stellar environment of SMC N81.
o	parag.3.2: background galaxy = EQ J010925.8-731155.9 in SIMBAD.
o	Table 1, parag.3.2: <[HMC2003b] NNN> N=42 among 519.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMC2007]
[HMC2007]	(Henry+Malkan+Colbert+, 2007)
Write:	<<[HMC2007] NN>>
N:	14
Object:	Poss. LBG (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST NICMOS Parallel Imaging Survey observations of Lyman Break Galaxy candidates.
Ref:	=2007ApJ...656L...1H
by	HENRY A.L. , MALKAN M.A., COLBERT J.W., SIANA B., TEPLITZ H.I., McCARTHY P., YAN L.
	Astrophys. J., 656L, 1-4 (2007)
	A search for Lyman break galaxies at z>8 in the NICMOS Parallel Imaging Survey.
o	Table 1: <[HMC2007] NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMC2008]
[HMC2008]	(Henry+Malkan+Colbert+, 2008)= (JD)
Write:	<<[HMC2008] JD JHHMM+DDMM>>
N:	1
Object:	Poss. LBG (SIMBAD class: Galaxy)
Note:	Discovery of a z about 9 Lyman break galaxy candidate, selected from the HST NICMOS Parallel Imaging Survey. Use of Spitzer IRAC photometry.
Ref:	=2008ApJ...680L..97H
by	HENRY A.L. , MALKAN M.A., COLBERT J.W., SIANA B., TEPLITZ H.I., McCARTHY P.
	Astrophys. J., 680L, 97-100 (2008)
	A Lyman break galaxy candidate at z ~ 9.
o	Text: <[HMC2008] JD JHHMM+DDMM> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMC2016]
[HMC2016]	(Hatch+Muldrew+Cooke+, 2016)
Write:	<<[HMC2016] Group N>> <<[HMC2016] Field group A>>
N:	8 (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS and HAWK-I observations of N=6+2 galaxy groups in the field of the Cl 0218.3-0510 protocluster at z=1.623.
in source:	ClG J0218-0510
Ref:	=2016MNRAS.459..387H
by	HATCH N.A. , MULDREW S.I., COOKE E.A., HARTLEY W.G., ALMAINI O., SIMPSON C.J., CONSELICE C.J.
	Mon. Not. R. Astron. Soc., 459, 387-401 (2016)
	The structure and evolution of a forming galaxy cluster at z = 1.62.
o	Table 2: <[HMC2016] Group N> (Nos 1-6), <[HMC2016] Field group A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMC99]
[HMC99]	(Hearty+Magnani+Caillault+, 1999)= ([MNC99a])
Write:	<<[HMC99] RX JHHMM.m+DDMMa>>
N:	42
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	ROSAT All-Sky survey of MBM 7 and MBM 55. Table 3: possible counterparts of the RX. When there are several possible counterparts for the same RX, they are '[HMC99] RX JHHMM.m+DDMMa'. See also [AKS95b], [ATW96], [WKS96], [CAA97], KWS97], [MMS97], [KWS97], [HMC99].
Ref:	=1999A&A...341..163H
by	HEARTY T. , MAGNANI L., CAILLAULT J.-P., NEUHAEUSER R., SCHMITT J.H.M.M., STAUFFER J.
	Astron. Astrophys., 341, 163-None (1999)
	A search for star formation in the translucent clouds MBM 7 and MBM 55.
o	Table 1 : misprint in the coordinates of RX J0344.9+0359 (α = 3 44 53).
o	Table 3: <[HMC99] RX JHHMM.m+DDMMa> N=42.
=E=	Catalogue in electronic form as J/A+A/341/163
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMC99a]
[HMC99a]	(Hearty+Magnani+Caillault+, 1999)
*****	Avoid the usage of [HMC99a], prefer [HMC99]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMC99b]
[HMC99b]	(Hu+McMahon+Cowie, 1999)= (HCM)
Write:	<<[HMC99b] SSA22-HCM1>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Note:	N=1 high redshift Ly alfa emitting galaxy in Hawaii narrowband survey. LRIS observations on Keck II. Field SSA 22.
Ref:	=1999ApJ...522L...9H
by	HU E.M. , McMAHON R.G., COWIE L.L.
	Astrophys. J., 522, 9-12 (1999)
	An extremely luminous galaxy at z = 5.74.
o	<[HMC99b] SSA22-HCM1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMD2012]
[HMD2012]	(Henry+Martin+Dressler+, 2012)
Write:	<<[HMD2012] NNN.N+N+N.NN>>
N:	6+21
Object:	LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	Magellan-Baade Telescope IMACS and Keck DEIMOS spectroscopic observations of ultra-faint emission-line galaxies.
Ref:	=2012ApJ...744..149H
by	HENRY A.L. , MARTIN C.L., DRESSLER A., SAWICKI M., McCARTHY P.
	Astrophys. J., 744, 149 (2012)
	The faint-end slope of the redshift 5.7 Lyα luminosity function.
o	Table 2: <[HMD2012] NN.N+N+N.NN> N=6.
Ref:	=2013ApJ...769..148H
by	HENRY A. , MARTIN C.L., FINLATOR K., DRESSLER A.
	Astrophys. J., 769, 148 (2013)
	The metallicity evolution of low-mass galaxies: new constraints at intermediate redshift.
o	Tables 2-3: <[HMD2012] NNN.N+N+N.NN> N=21 added, <MSDM NNN.N+N.N> (No. 28.0+7.1) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMD92]
[HMD92]	(Holmgren+McCausland+Dufton+, 1992)
Write:	<<[HMD92] FFF-NN>>
N:	50
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=49 stars, in fields 789 to 867, from the UKST UBVRI survey.
Ref:	=1992MNRAS.258..521H
by	HOLMGREN D.E. , McCAUSLAND R.J.H., DUFTON P.L., KEENAN F.P., KILKENNY D.
	Mon. Not. R. Astron. Soc., 258, 521-526 (1992)
	Low-dispersion spectroscopy of blue stars from UK Schmidt Telescope UBVRI survey.
o	<[HMD92] FFF-NN> N=50
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HMDS
HMDS	(Hawai Medium Deep Survey)
Write:	<<HMDS SSA-NN NNN>> <<HMDS DUR-NN NNN>>
N:	396
Object:	* or G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Tables 11-17: In the format the letters 'SSA' stands for 'SSA' fields of Hawai Deep Survey, 'DUR' for Durnham LDSS fields.
Ref:	=1995ApJS...98..441G
by	GARDNER J.P.
	Astrophys. J., Suppl. Ser., 98, 441-475 (1995)
	A near-infrared faint galaxy survey : the catalog.
o	<HMWS SSA-NN NNN> N=89+121+131+135+152, <HMWS DUR-NN NNN> N=123, <HMDS DUR-NN> N=119, <HMDS SSA-NN NNN> N=154+70+53+24+64+125
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HME2010]
[HME2010]	(Horesh+Maos+Ebeling+, 2010)
Write:	<<[HME2010] MACS JHHMM.m+DDMM AN>> <<[HME2010] RCS JHHMMSS+DDMM.m A>> <<[HME2010] RCSHHMMSS+DDMM.m A>> (not recognised by Simbad, but found in literature)
N:	49
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	Use of HST ACS archival data to study lensed arcs in galaxy clusters.
Ref:	=2010MNRAS.406.1318H
by	HORESH A. , MAOZ D., EBELING H., SEIDEL G., BARTELMANN M.
	Mon. Not. R. Astron. Soc., 406, 1318-1336 (2010)
	The lensing efficiencies of MACS X-ray-selected versus RCS optically selected galaxy clusters.
o	Fig. 1, Table 6: <[HME2010] MACS JHHMM.m+DDMM AN>, <[HME2010] RCS JHHMMSS+DDMM.m A>, N=49.
o	Cl 0024+24 is a misprint for ClG 0024+16
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HMEN
HMEN	(Henize+Mendoza)
*****	Avoid the usage of HMEN, prefer Ass Cha T
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HMF2009]
[HMF2009]	(Huang+Morokuma+Fakhouri+, 2009)
Write:	<<[HMF2009] NN>> <<[HMF2009] A>> <<[HMF2009] WARPS J1415.1+3612 lens>>
N:	25+7
Object:	G + Grav. lensed image of a G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST ACS photometry and Subaru FOCAS observations of the strong lensing cluster of galaxies WARPS J1415+3611.
in source:	WARPS J1415.0+3612
Ref:	=2009ApJ...707L..12H
by	HUANG X. , MOROKUMA T., FAKHOURI H.K., ALDERING G., AMANULLAH R., BARBARY K., BRODWIN M., CONNOLLY N.V., DAWSON K.S., DOI M., FACCIOLI L., FADEYEV V., FRUCHTER A.S., GOLDHABER G., GLADDERS M.D., HENNAWI J.F., IHARA Y., JEE M.J., KOWALSKI M., KONISHI K., LIDMAN C., MEYERS J., MOUSTAKAS L.A., PERLMUTTER S., RUBIN D., SCHLEGEL D.J., SPADAFORA A.L., SUZUKI N., TAKANASHI N., YASUDA N.
	Astrophys. J., 707L, 12-16 (2009)
	Hubble space telescope discovery of a z = 3.9 multiply imaged galaxy behind the complex cluster lens WARPS J1415.1+36 at z = 1.026.
o	Fig. 1, Table 1: <[HMF2009] NN> (Nos 1-25), <[HMF2009] A> (Nos A-G), <[HMF2009] WARPS J1415.1+3612 lens> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMG2003]
[HMG2003]	(Hjorth+Moller+Gorosabel+, 2003)
Write:	<<[HMG2003] GRB 020124 abs N.NNN>>
N:	1
Object:	DLA
Note:	The burst of GRB 020124 occured in a very faint Damped Lyman-Alpha Absorber at a redshift 3.198.
Ref:	=2003ApJ...597..699H
by	HJORTH J. , MOLLER P., GOROSABEL J., FYNBO J.P.U., TOFT S., JAUNSEN A.O., KAAS A.A., PURSIMO T., TORII K., KATO T., YAMAOKA H., YOSHIDA A., THOMSEN B., ANDERSEN M.I., BURUD I., CASTRO CERON J.M., CASTRO-TIRADO A.J., FRUCHTER A.S., KAPER L., KOUVELIOTOU C., MASETTI N., PALAZZI E., PEDERSEN H., PIAN E., RHOADS J., ROL E., TANVIR N.R., VREESWIJK P.M., WIJERS R.A.M.J., VAN DEN HEUVEL E.P.J.
	Astrophys. J., 597, 699-705 (2003)
	Very high column density and small reddening toward GRB 020124 at z=3.20.
o	Text: <[HMG2003] GRB 020124 abs 3.198> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMH2002]
[HMH2002]	(Howell+Mason+Huber+, 2002)
Write:	<<[HMH2002] HA JHHMM+DDMM>>
N:	12
Object:	Poss. Catacl. V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	ESO NTT observations to search for faint variable sources N=25 cataclysmic variable candidates, among which 12 H-alpha candidates (others are FSVS). See also FSVS.
Ref:	=2002A&A...395L..47H
by	HOWELL S.B. , MASON E., HUBER M., CLOWES R.
	Astron. Astrophys., 395, 47-50 (2002)
	Discovery of two new faint cataclysmic variables.
o	The two new CV* are [HMH2002] HA J0242-2802 and FSVS J1722+2723.
o	Table 1: <FSVS JHHMM+DDMM> N=13. Table 1: <[HMH2002] HA JHHMM+DDMM> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMH2007]
[HMH2007]	(Harvey+Merin+Huard+, 2007)
Write:	<<[HMH2007] NNN>> <<[HMH2007] JHHMMSS.s+DDMMSS>>
N:	286+1
Object:	YSO + Poss. YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	SST MIPS and IRAC observations of the Serpens Cloud.
in source:	NAME Serpens Cloud
Ref:	=2007ApJ...663.1149H
by	HARVEY P. , MERIN B., HUARD T.L., REBULL L.M., CHAPMAN N., EVANS II N.J., MYERS P.C.
	Astrophys. J., 663, 1149-1173 (2007)
	The Spitzer c2d survey of large, nearby, interstellar clouds. IX. The Serpens YSO population as observed with IRAC and MIPS.
o	Tables 2,3: <[HMH2007] NNN> (Nos 1-286). Par. 3.2: <[HMH2007] J182957.4+003141>.
=E=	Catalogue in electronic form as J/ApJ/663/1149
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMH2016]
[HMH2016]	(Hong+Mori+Hailey+, 2016)
Write:	<<[HMH2016] NN>>
N:	70+7
Object:	(Hard X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	NuSTAR observations of N=70+7 hard X-ray point sources in the 0.6deg² region around the Galactic Center and in the field of Sgr B2 cloud.
in source:	NAME Galactic Center
in source:	NAME Sgr B2
Ref:	=2016ApJ...825..132H
by	HONG J. , MORI K., HAILEY C.J., NYNKA M., ZHANG S., GOTTHELF E., FORNASINI F.M., KRIVONOS R., BAUER F., PEREZ K., TOMSICK J.A., BODAGHEE A., CHIU J.-L., CLAVEL M., STERN D., GRINDLAY J.E., ALEXANDER D.M., ARAMAKI T., BAGANOFF F.K., BARRET D., BARRIERE N., BOGGS S.E., CANIPE A.M., CHRISTENSEN F.E., CRAIG W.W., DESAI M.A., FORSTER K., GIOMMI P., GREFENSTETTE B.W., HARRISON F.A., HONG D., HORNSTRUP A., KITAGUCHI T., KOGLIN J.E., MADSEN K.K., MAO P.H., MIYASAKA H., PERRI M., PIVOVAROFF M.J., PUCCETTI S., RANA V., WESTERGAARD N.J., ZHANG W.W., ZOGLAUER A.
	Astrophys. J., 825, 132-132 (2016)
	NuSTAR hard X-ray survey of the Galactic Center region. II. X-ray point sources.
o	Tables 2-5: <[HMH2016] NN> (Nos 1-77).
=E=	Catalogue in electronic form as J/ApJ/825/132
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMH72]
[HMH72]	(Hoskins+Murdoch+Hazard+, 1972) (Not yet in Simbad)
Write:	<<[HMH72] HHMM+DD.da>>
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Identif. charts
Ref:	=1972AuJPh..25..559H
by	HOSKINS D.G. , MURDOCH H.S., HAZARD C., JAUNCEY D.L.
	Australian J. Phys., 25, 559-579 (1972)
	Positions and some identifications for 111 sources of about 1 flux unit at 408MHz.
o	Table 1: <[HMH72] HHMM+DDd> N=111
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMI96]
[HMI96]	(Hook+McMahon+Iwin+, 1996)= (GB)
Write:	<<[HMI96] HHMM+DDMM>>
N:	179
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1996MNRAS.282.1274H
by	HOOK I.M. , McMAHON R.G., IRWIN M.J., HAZARD C.
	Mon. Not. R. Astron. Soc., 282, 1274-1298 (1996)
	A survey for high-redshift radio-loud quasars : optical spectroscopy of S > 0.2 Jy, flat-spectrum radio sources.
o	Tables 1, 3, 4, 5: <[HMI96] HHMM+DDMM> N=179
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMK94]
[HMK94]	(Harrison+McNamara+Klemola, 1994)= ([HMK94a])
Write:	<<[HMK94] NN>>
N:	98
Object:	* (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Nos 4, 6, 17 35, 92 and 95 are not stars but galaxies.
Ref:	=1994AJ....107..254H
by	HARRISON T.E. , McNAMARA B.J., KLEMOLA A.R.
	Astron. J., 107, 254-260 (1994)
	Optical studies of γ-ray burst fields. I. GRB 790329.
o	[HMK94] 8 = ADS 7798AB, not 7795AB as quoted in the text p. 258
o	<[HMK94] NN> N=98
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMK94a]
[HMK94a]	(Harrison+McNamara+Klemola, 1994)
*****	Avoid the usage of [HMK94a], prefer [HMK94]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMK94b]
[HMK94b]	(Harrison+McNamara+Klemola, 1994)
Write:	<<[HMK94b] 1-NN>> <<[HMK94b] 2-NN>>
N:	60+58
Object:	Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 1: format '1-NN', N=60 obj. in the error box of GRB 790613. Table 2: format '2-NN', N=58 obj. in the error box of GRB 781124.
Ref:	=1994AJ....108..600H
by	HARRISON T.E. , McNAMARA B.J., KLEMOLA A.R.
	Astron. J., 108, 600-604 (1994)
	Optical studies of γ-ray burst fields. III. GRB 790613 and GRB 781124.
o	Table 1: <[HMK94b] 1-NN> N=60. Table 2: <[HMK94b] 2-NN> N=58
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HML2019]
[HML2019]	(HOLLYHEAD+MARTOCCHIA+LARDO+, 2-19)
Write:	<<[HML2019] NNNNN>>
N:	37
Object:	* (SIMBAD class: Star)
Note:	VLT FORS2 spectroscopic observations of N=37 stars in the globular cluster Hodge 6 in the LMC.
in source:	[H60b] 6
Ref:	=2019MNRAS.484.4718H
by	HOLLYHEAD K. , MARTOCCHIA S., LARDO C., BASTIAN N., KACHAROV N., NIEDERHOFER F., CABRERA-ZIRI I., DALESSANDRO E., MUCCIARELLI A., SALARIS M., USHER C.
	Mon. Not. R. Astron. Soc., 484, 4718-4725 (2019)
	Spectroscopic detection of multiple populations in the ~2 Gyr old cluster Hodge 6 in the LMC.
o	Table 1: <[HML2019] NNNNN> N=37 among (Nos 3581-20569).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMM2016]
[HMM2016]	(Hinojosa-Goni+Munoz-Tunon+Mendez-Abreu, 2016) (Not yet in Simbad)
Write:	<<[HMM2016] cosmos-NNN>> <<[HMM2016] cosmos-NNN N>>
N:	220+306
Object:	Starburst G + Knot (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=220 starburst galaxies in the COSMOS field and N=306 star-forming knots in those 220 starburst galaxies. Use of COSMOS data from the photometric redshift catalogue ([ICS2009]), the COSMOS intermediate and broadband photometric catalogue (COSMOS), and the spectra available in zCOSMOS.
in source:	NAME COSMOS Field
Ref:	=2016A&A...592A.122H
by	HINOJOSA-GONI R. , MUNOZ-TUNON C., MENDEZ-ABREU J.
	Astron. Astrophys., 592A, 122-122 (2016)
	Starburst galaxies in the COSMOS field: clumpy star-formation at redshift 0 <z < 0.5.
o	Table 3: <[HMM2016] COSMOS-NNN> (Nos 001-220). Table 4: <[HMM2016] COSMOS-NNN N> N=306.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMM90]
[HMM90]	(Heydari-Malayeri+Melnick+Martin, 1990)
Write:	<<[HMM90] AN>> <<[HMM90] A>>
N:	2+4
Object:	HII + Part of G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=2 (Nos A1-A2) giant HII regions in IC 4662 N=4 components (Nos A-D) of IC 4662. See also [JIP2003].
in source:	IC 4662
Ref:	=1990A&A...234...99H
by	HEYDARI-MALAYERI M. , MELNICK J., MARTIN J.M.
	Astron. Astrophys., 234, 99-105 (1990)
	Star formation in the irregular galaxy IC 4662.
o	<[HMM90] AN> (Nos A1-A2), <[HMM90] A> (Nos A-D)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMN98]
[HMN98]	(Hurley-Keller+Mateo+Nemec, 1998)
Write:	<<[HMN98] N-NNNN>>
N:	3051+2233+2025
Object:	* (SIMBAD class: Star)
Note:	Photometry in 3 fields (Nos 1-3) in Carina dw galaxy. See also [MHN98]
in source:	NAME Carina Dwarf Galaxy
Ref:	=1998AJ....115.1840H
by	HURLEY-KELLER D. , MATEO M., NEMEC J.
	Astron. J., 115, 1840-1855 (1998)
	The star formation history of the Carina dwarf galaxy.
o	Table 2: <[HMN98] N-NNNN> N=3051+2233+2025.
=E=	Catalogue in electronic form as J/AJ/115/1840
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMP2006]
[HMP2006]	(Henze+Meusinger+Pietsch, 2006)
Write:	<<[HMP2006] NN>>
N:	19
Object:	Poss. Nova (SIMBAD class: Nova = Classical Nova)
Stat:	is completely incorporated in Simbad
Note:	Tautenburg Schmidt telescope UBV photometry. Search for new possible novae in M 31. (Nos 1-32) were previously catalogued and are not published in 2006IBVS.5739....1H. See also M31N.
in source:	M 31 = NGC 224
Ref:	=2006IBVS.5739....1H
by	HENZE M. , MEUSINGER H., PIETSCH W.
	IAU Inform. Bull. Var. Stars, 5739, 1-4 (2006)
	Discovery of 19 new historical nova candidates in M 31.
o	Table 1: <[HMP2006] NN> (Nos 33-51).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMP93]
[HMP93]	(Hamuy+Maza+Phillips+, 1993)
Write:	<<[HMP93] SN 1990S N>> <<[HMP93] SN 1990T N>> <<[HMP93] SN 1990Y N>> <<[HMP93] SN 1990af NN>>
N:	8+8+9+14
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 5: * around SN 1990S, N=8. Table 8: * around SN 1990T, N=8. Table 11: * around SN 1990Y, N=9. Table 13: * around SN 1990af, N=12, (Nos 1-14), Nos 7 and 11 are missing. See also [HPM94] and [HPS96]
Ref:	=1993AJ....106.2392H
by	HAMUY M. , MAZA J., PHILLIPS M.M., SUNTZEFF N.B., WISCHNJEWSKY M., SMITH R.C., ANTEZANA R., WELLS L.A., GONZALEZ L.E., GIGOUX P., NAVARETTE M., BARRIENTOS F., LAMONTAGNE R., DELLA VALLE M., ELIAS J.E., PHILLIPS A.C., ODEWAHN S.C., BALDWIN J.A., WALKER A.R., WILLIAMS T., STURCH C.R., BAGANOFF F.K., CHABOYER B.C., SCHOMMER R.A., TIRADO H., HERNANDEZ M., UGARTE P., GUHATHAKURTA P., HOWELL S.B., SZKODY P., SCHMIDTKE P.C., ROTH J.
	Astron. J., 106, 2392-2407 (1993)
	The 1990 Calan/Tololo supernova search.
o	Table 5: <[HMP93] SN 1990S N> N=8, Table 8: <[HMP93] SN 1990T N > N=8, Table 11: <[HMP93] SN 1990Y N> N=9, Table 13: <[HMP93] SN 1990af NN> N=14
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMR2009]
[HMR2009]	(Harris+Mouhcine+Rejkuba+, 2009)
Write:	<<[HMR2009] GNN>>
N:	43
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Stat:	is completely incorporated in Simbad
Note:	HST ACS photometry of N=43 globular cluster candidates in NGC 891.
in source:	NGC 891
Ref:	=2009MNRAS.395..436H
by	HARRIS W.E. , MOUHCINE M., REJKUBA M., IBATA R.
	Mon. Not. R. Astron. Soc., 395, 436-442 (2009)
	Globular cluster candidates in NGC 891.
o	Table 1: <[HMR2009] GNN> (Nos G01-G43).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMR2011]
[HMR2011]	(Hibon+Malhotra+Rhoads+, 2011)= (LAE)
Write:	<<[HMR2011] LAE N>>
N:	6
Object:	LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Magellan Baade 6.5m telescope IMACS narrow-band observations of the COSMOS field.
in source:	NAME COSMOS Field
Ref:	=2011ApJ...741..101H
by	HIBON P. , MALHOTRA S., RHOADS J., WILLOTT C.
	Astrophys. J., 741, 101 (2011)
	Search for z ~ 6.96 Lyα emitters with Magellan/IMACS in the COSMOS field.
o	Table 3: <[HMR2011] LAE N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMR2016]
[HMR2016]	(Hoffmann+Macri+Riess+, 2016)
Write:	<<[HMR2016] {M101\|U9391} NNNNNNN>> <<[HMR2016] NNNNN NNNNNNN>> <<[HMR2016] {N\|U}NNNN {H}NNNa>> <<[HMR2016] {N\|U}NNNN {N}NN>> <<[HMR2016] N3982 HNN>>
N:	3048+171+14+2
Object:	* + Cepheid + HII (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=1095 standard stars, N=1956 Cepheids, and N=171+14+2 HII regions in 20 galaxies, as part of the SH0ES project (Supernovae and H0 for the Equation of State of dark energy) for Cepheid variable stars. Use of HST WFPC2/ACS/WFC observations.
Ref:	=2016ApJ...830...10H
by	HOFFMANN S.L. , MACRI L.M., RIESS A.G., YUAN W., CASERTANO S., FOLEY R.J., FILIPPENKO A.V., TUCKER B.E., CHORNOCK R., SILVERMAN J.M., WELCH D.L., GOOBAR A., AMANULLAH R.
	Astrophys. J., 830, 10-10 (2016)
	Optical identification of cepheids in 19 host galaxies of Type Ia supernovae and NGC 4258 with the Hubble Space Telescope.
o	Tables 3+5: <[HMR2016] ANNNN NNNNNNN> N=1095+1956. Table 7: <[HMR2016] ANNNN HNNNa> N=171, <[HMR2016] ANNNN NNN> N=14,<[HMR2016] N3982 HNN> (Nos N3982 HN1-N3982 HN2).
=E=	Catalogue in electronic form as <J/ApJ/830/10/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMR80]
[HMR80]	(Haschick+Moran+Rodriguez+, 1980)
Write:	<<[HMR80] H2O(A)>>
N:	5
Object:	Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	N=5 masers in the vicinity of HH 7-11 objects (NGC 1333), the 1st maser was already known before 1980.
in source:	NGC 1333
Ref:	=1980ApJ...237...26H
by	HASCHICK A.D. , MORAN J.M., RODRIGUEZ L.F., BURKE B.F., GREENFIELD P., GARCIA-BARRETO J.A.
	Astrophys. J., 237, 26-37 (1980)
	Observations of a compact H II region and water vapor maser sources in the vicinity of the Herbig-Haro objects 7-11.
o	Table 1: <[HMR80] H2O(A)> (Nos (A), (B), (C)).
Ref:	=1986A&A...165..197H
by	HENKEL C. , HASCHICK A.D., GUSTEN R.
	Astron. Astrophys., 165, 197-203 (1986)
	H2O maser emission from HH 6 and other star-forming regions.
o	Table 1: <[HHG86] HHMMSS.s+DDMMSS> N=19. Table 1: <[HMR80] H2O(D)> added.
Ref:	=1988A&A...192..153L
by	LISEAU R. , SANDELL G., KNEE L.B.G.
	Astron. Astrophys., 192, 153-164 (1988)
	The structure of the molecular outflow near SSV 13 and HH 7-11 in the NGC 1333 region.
o	Fig.1a: <[HMR80] H2O(E)> added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMR88]
[HMR88]	(Heydari-Malayeri+Magain+Remy, 1988)
Write:	<<[HMR88] Sk -66 41 a>>
N:	6
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Sk -66 41 is a multiple system, called 'Sk -66 41 Cluster' by the the authors. See also [HB94], [HRR2000].
in source:	NAME SK -66 41 Cluster
Ref:	=1988A&A...201L..41H
by	HEYDARI-MALAYERI M. , MAGAIN P., REMY M.
	Astron. Astrophys., 201, 41-43 (1988)
	New evidence against the existence of very massive stars.
o	<NAME SK -66 41 CLUSTER>. Table 2: <[HMR88] Sk -66 41 a> (Nos a-f).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HMS
HMS	(Humason+Mayall+Sandage)= (Cl)
Write:	<<HMS HHMM+DDMMA>>
N:	439
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	The 'HMS' designation from 1st ref. is extended to all clusters (N=439) in the 3rd ref.
Ref:	=1956AJ.....61...97H
by	HUMASON M.L. , MAYALL N.U., SANDAGE A.R.
	Astron. J., 61, 97-162 (1956)
	Redshifts and magnitudes of extragalactic nebulae.
o	Table I: <[HMS56] Anon HHMM.m+DDMM> N=17. Table III: <HMS HHMM+DDMMA> N=21. Table III, Plates I, II: <[HMS56] HHMM+DDMM NNA> N=124
Ref:	=1973AJ.....78...26N
by	NOONAN T.W.
	Astron. J., 78, 26-31 (1973)
	List of clusters of galaxies with published redshifts.
o	<HMS HHMM+DDMMA> N=138
Ref:	=1981ApJS...45..613N
by	NOONAN T.W.
	Astrophys. J., Suppl. Ser., 45, 613-620 (1981)
	List of clusters of galaxies with published redshifts.
o	Table 1: <HMS HHMM+DDMMA> N=439
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HMS2009]
[HMS2009]	(Hayashi+Motohara+Shimasaku+, 2009)= (BzK) = (sBzK)
Write:	<<[HMS2009] NNNNN>>
N:	15
Object:	G (SIMBAD class: Galaxy)
Note:	Multi-Object IR Camera and Spectrograph (MOIRCS) on the Subaru telescope observations to search for star-forming BzK galaxies.
Ref:	=2009ApJ...691..140H
by	HAYASHI M. , MOTOHARA K., SHIMASAKU K., ONODERA M., UCHIMOTO Y.K., KASHIKAWA N., YOSHIDA M., OKAMURA S., LY C., MALKAN M.A.
	Astrophys. J., 691, 140-151 (2009)
	Star formation rates and metallicities of k-selected star-forming galaxies at z ~ 2.
o	Fig.2, Tables 1, 2: <[HMS2009] NNNNN> N=15 among (Nos 21193-31569).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMS2010]
[HMS2010]	(Hennawi+Myers+Shen+, 2010)
Write:	<<[HMS2010] SDSS JHHMM+DDMMA>> <<[HMS2010] PSS JHHMM+DDMMA>>
N:	27*2
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	ARC 3.5m telescope, 6.5m MMT, Palomar 200inch telescope, and Kitt Peak Mayall 4m telescope spectroscopy of high-redshift binary quasars. Use of SDSS data. See also [HSO2006], [MRB2008].
Ref:	=2010ApJ...719.1672H
by	HENNAWI J.F. , MYERS A.D., SHEN Y., STRAUSS M.A., DJORGOVSKI S.G., FAN X., GLIKMAN E., MAHABAL A., MARTIN C.L., RICHARDS G.T., SCHNEIDER D.P., SHANKAR F.
	Astrophys. J., 719, 1672-1692 (2010)
	Binary quasars at high redshift. I. 24 new quasar pairs at z ~ 3-4.
o	Table 3: <[HMS2010] SDSS JHHMM+DDMMA>, <[HMS2010] PSS JHHMM+DDMMA> N=27*2.
=E=	Catalogue in electronic form as <J/ApJ/719/1672/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMS56]
[HMS56]	(Humason+Mayall+Sandage, 1956)
Write:	<<[HMS56] Anon HHMM.m+DDMM>> <<[HMS56] HHMM+DDMM NNA>>
N:	17+124
Object:	G (SIMBAD class: Galaxy)
Note:	In the same ref. 1956AJ.....61...97H Table III are the N=21 first HMS ClG. Table I: N=17 galaxies, named 'Anon' by the authors, format 'Anon HHMM.m+DDMM'. Table III and Plates I, II: N=124 galaxies in the 21 HMS clusters, format 'HHMM+DDMM NNA' where 'HHMM+DDMM' stands for the HMS ClG format.
Ref:	=1956AJ.....61...97H
by	HUMASON M.L. , MAYALL N.U., SANDAGE A.R.
	Astron. J., 61, 97-162 (1956)
	Redshifts and magnitudes of extragalactic nebulae.
o	Table I: <[HMS56] Anon HHMM.m+DDMM> N=17. Table III: <HMS HHMM+DDMMA> N=21. Table III, Plates I, II: <[HMS56] HHMM+DDMM NNA> N=124
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMS93]
[HMS93]	(Hillenbrand+Massey+Strom+, 1993)
Write:	<<[HMS93] JHHMMSS.ss+DDMMSS.s>>
N:	1022
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Observations made at the Kitt Peak National Observatory. Optical CCD photometry and spectroscopy is combined with NIR imaging photometry to study the young cluster NGC 6611.
in source:	NGC 6611 = Eagle Nebula = M 16
Ref:	=1993AJ....106.1906H
by	HILLENBRAND L.A. , MASSEY P., STROM S.E., MERRILL K.M.
	Astron. J., 106, 1906-1946 (1993)
	NGC 6611: a cluster caught in the act.
o	Table 1: <[HMS93] JHHMMSS.ss+DDMMSS.s> N=1022.
=E=	Catalogue in electronic form as J/AJ/106/1906
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMS95]
[HMS95]	(Hillenbrand+Meyer+Strom+, 1995)
Write:	<<[HMS95] NNN>>
N:	33+6
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-33) and N=6 among (Nos 118-140)
in source:	NAME BD +40 4124 Cluster
Ref:	=1995AJ....109..280H
by	HILLENBRAND L.A. , MEYER M.R., STROM S.E., SKRUTSKIE M.F.
	Astron. J., 109, 280-297 (1995)
	Isolated star-forming regions containing Herbig Ae/Be stars. I. The young stellar aggregate associated with BD +40 4124.
o	p. 297: Red nebular source = EQ J202047+411216
o	Tables 1-2: <[HMS95] NNN> (Nos 1-33) and N=6 among (Nos 118-140). <Em* LkHA NNNW> (Nos 225N, 225S).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HMST
HMST	(Hartley+Manchester+Smith+Tritton)= (DC) = (HMSTG)
Write:	<<HMST LLL.l+BB.b>>
N:	1101
Object:	Dark Cloud + Globule (SIMBAD class: DarkNeb = Dark Cloud (nebula))
Note:	ESO-SERC survey for declinations south of -33deg. Catalogue of 1101 dark clouds.
Ref:	=1986A&AS...63...27H
by	HARTLEY M. , MANCHESTER R.N., SMITH R.M., TRITTON S.B., GOSS W.M.
	Astron. Astrophys., Suppl. Ser., 63, 27-48 (1986)
	A catalogue of southern dark clouds.
o	Table 1: <HMST LLL.l+BB.b> N=1101.
=E=	Catalogue in electronic form as VII/68
Origin	of the Acronym: L (2002A&A...383..631D)
Details on Acronym: HMSTG
HMSTG	(Hartley+Manchester+Smith+Tritton, Globule)
*****	Avoid the usage of HMSTG, prefer HMST
Origin	of the Acronym: L (2002A&A...383..631D)
Details on Acronym: [HMT84]
[HMT84]	(Hazard+Morton+Terlevich+, 1984)= (H)
Write:	<<[HMT84] HHMM+DDd>>
N:	9
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Ref:	=1984ApJ...282...33H
by	HAZARD C. , MORTON D.C., TERLEVICH R., McMAHON R.
	Astrophys. J., 282, 33-52 (1984)
	Nine new quasi-stellar objects with broad absorption lines.
o	Table 1: <[HMT84] HHMM+DDd> N=9
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMT98]
[HMT98]	(Hunt+Mannucci+Testi+, 1998)= (AS)
Write:	<<[HMT98] AS NN-N>>
N:	86
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	In the format 'AS' stands for ARNICA Standard, the two first digits 'NN' for fields 01 to 40, and the last digit 'N' for a running number in each field. This last digit is '0' for the central star in each field. Fig.1: Finding Charts.
Ref:	=1998AJ....115.2594H
by	HUNT L.K. , MANNUCCI F., TESTI L., MIGLIORINI S., STANGA R.M., BAFFA C., LISI F., VANZI L.
	Astron. J., 115, 2594-2603 (1998)
	Northern JHK standard stars for array detectors.
o	(Erratum) Erratum vol. 119, p. 985 (2000)
o	Table 1: <[HMT98] AS NN-N> N=86
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMU2001]
[HMU2001]	(Hirano+Mikami+Umemoto+, 2001)= (Hi2000)
Write:	<<[HMU2001] IRAS 16293-2422 WN>>
N:	4
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	SiO emission clumps associated with the outflow driven by IRAS 16293-2422. See also [CCL2001].
in source:	IRAS 16293-2422
Ref:	=2001ApJ...547..899H
by	HIRANO N. , MIKAMI H., UMEMOTO T., YAMAMOTO S., TANIGUCHI Y.
	Astrophys. J., 547, 899-906 (2001)
	SiO emission in the multilobe outflow associated with IRAS 16293-2422.
o	Fig.1: <[HMU2001] IRAS 16293-2422 WN> (Nos E1-E2, W1-W2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HMV
HMV	(Heithausen+Mebold+de Vries)
Write:	<<HMV NN>>
N:	15
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Ref:	=1987A&A...179..263H
by	HEITHAUSEN A. , MEBOLD U., DE VRIES H.W.
	Astron. Astrophys., 179, 263-267 (1987)
	A survey of formaldehyde in high galactic latitudes.
o	<HMV NN> (Nos 1-15).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HMV93]
[HMV93]	(Hamuy+Maza+Valladares+, 1993)
Write:	<<[HMV93] HHMMSS+DDMM.m>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of SN 1993AG
Ref:	=1993IAUC.5895....1H
by	HAMUY M. , MAZA J., VALLADARES G., WISCHNJEWSKY M., ANTEZANA R., HO L.
	IAU Circ., 5895, 1-None (1993)
	Supernovae 1993af, 1993ag, 1993ah.
o	<[HMV93] HHMMSS+DDMM.m> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMW2003]
[HMW2003]	(Heydari-Malayeri+Meynadier+Walborn, 2003)
Write:	<<[HMW2003] NNN>>
N:	47+31
Object:	* in Cl* (SIMBAD class: Star)
Note:	Stars (Nos 1-14) are in the RMC 127 cluster, (Nos 15-47) are in the RMC 128 cluster, stars among (Nos 61-291) are the brightest stars in the field.
in source:	Magellanic Clouds:LMC:NAME RMC 127 CLUSTER = NAME RMC 127 CLUSTER
in source:	Magellanic Clouds:LMC:NAME RMC 128 CLUSTER = NAME RMC 128 CLUSTER
Ref:	=2003A&A...400..923H
by	HEYDARI-MALAYERI M. , MEYNADIER F., WALBORN N.R.
	Astron. Astrophys., 400, 923-937 (2003)
	Tight LMC massive star clusters R127 and R128.
o	Tables 1, 2, 3: <[HMW2003] NNN> (Nos 1-47) and N=31 among (Nos 61-291).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMW2016]
[HMW2016]	(Hu+Menten+Wu+, 2016)
Write:	<<[HMW2016] GLLL.lll+BB.bbb>>
N:	367
Object:	Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	VLA observations of N=367 6.7GHz methanol masers.
Ref:	=2016ApJ...833...18H
by	HU B. , MENTEN K.M., WU Y., BARTKIEWICZ A., RYGL K., REID M.J., URQUHART J.S., ZHENG X.
	Astrophys. J., 833, 18-18 (2016)
	On the relationship of UC HII regions and class II methanol masers. I. Source catalogs.
o	Table 3: <[HMW2016] GLLL.lll+BB.bbb> N=367.
=E=	Catalogue in electronic form as <J/ApJ/833/18/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMW82]
[HMW82]	(Herbst+Miller+Warner+, 1982) (Not yet in Simbad)
Write:	<<[HMW82] CMa R1 NN>> <<[HMW82] Mon R1 NN>> <<[HMW82] Simeis 188 NNW>> <<[HMW82] Simeis 188 NNa>> <<[HMW82] Simeis 188 NNaW>> <<[HMW82] M8-M20 N>> <<[HMW82] Vul R1 NN>> <<[HMW82] Vul R2 NNW>>
N:	32+19+19+7+17+19
Object:	* (SIMBAD class: Star)
Ref:	=1982AJ.....87...98H
by	HERBST W. , MILLER D.P., WARNER J.W., HERZOG A.
	Astron. J., 87, 98-121 (1982)
	R associations. VI. The reddening law in dust clouds and the nature of early-type emission stars in nebulosity from a study of five associations.
o	Table I: [HMW82] <CMa R1 NN> (Nos 1-32). Table II: <[HMW82] Mon R1 NN> (Nos 1-19). Table IV: <[HMW82] Simeis 188 NNW>, <[HMW82] Simeis 188 NNaW>, (Nos 1-17) N=19. Table V: <[HMW82] M8-M20 N> (Nos 1-7). Table VI: <[HMW82] Vul R1 NN> (Nos 1-17). Table VII: <[HMW82] Vul R2 NNW> (Nos 1-12, 13N, 13S, 14-18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMW88]
[HMW88]	(Harris+Dewdney+Costain+, 1988)
Write:	<<[HMW88] HHMM+DD RNN>> <<[HMW88] HHMM+DD XN>>
N:	119+11
Object:	(Rad) + (X) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Radio-sources and X-ray sources in 4 fields. Map of each field. See also Paper II: [DCM91]
Ref:	=1988ApJ...325..610H
by	HARRIS D.E. , DEWDNEY P.E., COSTAIN C.H., McHARDY I., WILLIS A.G.
	Astrophys. J., 325, 610-627 (1988)
	An X-ray and radio study of steep-spectrum radio sources. I. Four fields from the Clark Lake Observatory 26 MHz survey.
o	Table 2: <[HMW88] 0713+37 RNN> (Nos R1-R60). Table 3: <[HMW88] 0713+37 XN> (Nos X1-X5). Table 4: <[HMW88] 1244+26 RNN> (Nos R1-R24). Table 5: <[HMW88] 1530+41 RNN> (Nos R1-R16). Table 6: <[HMW88] 1530+41 XN> (Nos X1-X3). Table 7: <[HMW88] 1718+26 RNN> (Nos R1-R19). Table 8: <[HMW88] 1718+26 XN> (Nos X1-X3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HMW96]
[HMW96]	(Harrison+McNamara+Williams, 1996)
Write:	<<[HMW96] GRB910814 NN>> <<[HMW96] GRB910814 NN-N>> <<[HMW96] GRB920525 N>>
N:	39+41+4
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT PSPC and HRI observations. Table 1: ROSAT sources in the GRB 910814 error box. N=39 sources. Table 2: counterparts of the brighter x-ray sources in table 1. N=41, format 'NN-N'. Table 3: ROSAT sources in the GRB 920525 error box. N=4 sources. Paper II, see also Paper I: [MHW95]
Ref:	=1996AJ....112..216H
by	HARRISON T.E. , McNAMARA B.J., WILLIAMS C.L., WAGNER R.M.
	Astron. J., 112, 216-220 (1996)
	ROSAT observations of γ-ray burst error boxes. II. GRB 910814 and GRB 920525.
o	Table 1: <[HMW96] GRB910814 NN> (Nos 1-39). Table 2: <[HMW96] GRB910814 NN-N> N=41. Table 3: <[HMW96] GRB920525 N> (Nos 1-4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HMWS
HMWS	(Hawai Medium Wide Survey)
Write:	<<HMWS SSA-NN NNN>> <<HMWS DUR-NN NNN>>
N:	7511
Object:	* or G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Tables 5-10: In the format the letters 'AAA' stands for 'SSA' fields of Hawai Deep Survey, or for 'DUR' Durnham LDSS fields.
Ref:	=1995ApJS...98..441G
by	GARDNER J.P.
	Astrophys. J., Suppl. Ser., 98, 441-475 (1995)
	A near-infrared faint galaxy survey : the catalog.
o	<HMWS SSA-NN NNN> N=89+121+131+135+152, <HMWS DUR-NN NNN> N=123, <HMDS DUR-NN> N=119, <HMDS SSA-NN NNN> N=154+70+53+24+64+125
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HMxcl
HMxcl	(HectoMAP X-ray cluster)
Write:	<<HMxcl JHHMMSS.s+DDMMSS>>
N:	15
Object:	X-ray Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	N=15 X-ray clusters in the HectoMAP dense redshift survey of red galaxies, selected from the SDSS DR9.
Ref:	=2018ApJ...855..100S
by	SOHN J. , CHON G., BOHRINGER H., GELLER M.J., DIAFERIO A., HWANG H.S., UTSUMI Y., RINES K.J.
	Astrophys. J., 855, 100-100 (2018)
	The HectoMAP cluster survey. II. X-ray clusters.
o	Tables 1-2: <HMxcl JHHMMSS.s+DDMMSS> N=15.
=E=	Catalogue in electronic form as <J/ApJ/855/100/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HN
HN	(Hiltner Number)
*****	Avoid the usage of HN, prefer Hilt
Origin	of the Acronym: L (1971A&A....14..489H)
Details on Acronym: Hn
Hn	(Hartigan)
Write:	<<Hn NNW>>
N:	26+6
Object:	H-alpha obj. (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-26). Format 'NNW' introduced later Hn 10, 12, and 21 are double TTau* (This format first appears in 1996MNRAS.280.1071L).
in source:	NAME Cha I
in source:	NAME Cha II
Ref:	=1993AJ....105.1511H
by	HARTIGAN P.
	Astron. J., 105, 1511-1518 (1993)
	New T Tauri stars in Chamaeleon I and Chamaeleon II.
o	GK-1 = HBC 582
o	Table 3: <Hn NN> (Nos 1-26).
Ref:	=1998A&A...338..977C
by	CAMBRESY L. , COPET E., EPCHTEIN N., DE BATZ B., BORSENBERGER J., FOUQUE P., KIMESWENGER S., TIPHENE D.
	Astron. Astrophys., 338, 977-987 (1998)
	New young stellar object candidates in the Chamaeleon I molecular cloud discovered by DENIS.
o	Table 1: <[CCE98] 1-NNN> (Nos 1-1 to 1-126). Table 2: <[CCE98] 2-NN> (Nos 2-1 to 2-54). Table 1: <Hn NNW> (Nos 10E, 10W, 12E, 12W, 21E, 21W) added.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HN97]
[HN97]	(Hutchings+Neff, 1997)= ([HN97a])
Write:	<<[HN97] HHMM+DDd NN>> <<[HN97] HHMM+DD NN>> <<[HN97] HHMM+DDd NNA>> <<[HN97] HHMM+DDd A>> <<[HN97] HHMM+DDd Aa>>
N:	101
Object:	Non-stellar Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 2: N=101 non-stellar objects in 5 QSOs fields: Maps in figs 3, 6, 9, 11, 14. In the field 0052+252: format '0052+252 NN', (Nos 1-22), No. 13 = QSO 0052+252, cross-id. with '[BKS96b] PG 0052+251 A'. In the field 0453+22: format '0453+22 NN', (Nos 1-22), No. 12 is the RadioGalaxy 3C 132. In the field 0911+053: format '0911+053 NN', (Nos 1-18), No. 13 = QSO 0911+053, format '0911+053 Hs' = the Host galaxy, format '0911+053 12F' = its companion. In the field 0157+001: format '0157+001 NN', (Nos 1-17), Qnuc + Qtot = QSO 0157+001 = MRK 1014, format '0157+001 A', (Nos A-C) for 3 arms of the galaxy. In the field 0844+349: format '0844+349 NN', (Nos 1-14), No. Q = QSO 0844+349, format '0844+349 Hs' = the Host galaxy, format '0844+349 C' = its companion
Ref:	=1997AJ....113..550H
by	HUTCHINGS J.B. , NEFF S.G.
	Astron. J., 113, 550-561 (1997)
	JHK imaging and photometry of low z QSOs and radio galaxy.
o	Radiogalaxy 0453+22 = 3C 132
o	Table 2: <[HN97] HHMM+DDd NN>, <[HN97] HHMM+DD NN>, <[HN97] HHMM+DDd NNA>, <[HN97] HHMM+DDd A>, <[HN97] HHMM+DDd Hs>, N=101
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HN97a]
[HN97a]	(Hutchings+Neff, 1997)
*****	Avoid the usage of [HN97a], prefer [HN97]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HN97b]
[HN97b]	(Hutchings+Neff, 1997) (Not yet in Simbad)
Write:	<<[HN97b] NN>>
N:	21
Object:	* + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=3 stars + N=17 galaxies in the field of QSO 0820+296 (= [HN97b] 7)
Ref:	=1997AJ....113.1514H
by	HUTCHINGS J.B. , NEFF S.G.
	Astron. J., 113, 1514-1516 (1997)
	A QSO in a cluster at z=2.4.
o	Table 1: <[HN97b] NN> (Nos 1-21)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HNA97]
[HNA97]	(Hogg+Neugebauer+Armus+, 1997)
Write:	<<[HNA97] JHHMMSS.ss+DDMMSS.s>>
N:	88
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Near IR observations of Hubble Deep Field (HDF)
in source:	NAME HDFN
Ref:	=1997AJ....113..474H
by	HOGG D.W. , NEUGEBAUER G., ARMUS L., MATTHEWS K., PAHRE M.A., SOIFER B.T., WEINBERGER A.J.
	Astron. J., 113, 474-482 (1997)
	Near infrared imaging of the Hubble Deep Field with the Keck telescope.
o	(Erratum) Erratum AJ 113, p. 2338
o	Tables 1, 2: <[HNA97] JHHMMSS.ss+DDMMSS.s> N=44+44
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HNB98]
[HNB98]	(Hunter+Neugebauer+Benford+, 1998)
Write:	<<[HNB98] G34.24+0.13MM>> <<[HNB98] G34.24+0.13IR>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Ref:	=1998ApJ...493L..97H
by	HUNTER T.R. , NEUGEBAUER G., BENFORD D.J., MATTHEWS K., LIS D.C., SERABYN E., PHILLIPS T.G.
	Astrophys. J., 493, 97-100 (1998)
	G34.24+0.13MM: A deeply embedded proto-B-star.
o	Table 1: <[HNB98] G34.24+0.13MM>, <[HNB98] G34.24+0.13IR> N=2
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HNC2000]
[HNC2000]	(Hogg+Neugebauer+Cohen+, 2000)
Write:	<<[HNC2000] JHHMMSS.sss+DDMMSS.ss>>
N:	11
Object:	G + * (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	HDF images at 3.2micro.m taken with the Keck telescope. N=10 [WBD96] galaxies + 1 galactic star.
in source:	NAME HDFN
Ref:	=2000AJ....119.1519H
by	HOGG D.W. , NEUGEBAUER G., COHEN J.G., DICKINSON M., DJORGOVSKI S.G., MATTHEWS K., SOIFER B.T.
	Astron. J., 119, 1519-1525 (2000)
	3 micron imaging of the Hubble Deep Field.
o	Table 2: <[HNC2000] JHHMMSS.sss+DDMMSS.ss> N=11.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HNF99]
[HNF99]	(Heidt+Nilsson+Fried+, 1999) (Not yet in Simbad)
Write:	<<[HNF99] Galaxy A>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Note:	N=2 companions to the galaxy 1ES 1741+19.6
Ref:	=1999A&A...348..113H
by	HEIDT J. , NILSSON K., FRIED J.W., TAKALO L.O., SILLANPAEAE A.
	Astron. Astrophys., 348, 113-116 (1999)
	1ES 1741+196: a BL Lacertae object in a triplet of interacting galaxies?
o	MS 0419+197 = 1E 0419.3+1943
o	Table 1: <[HNF99] Galaxy A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HNM
HNM	(HDF NICMOS Mosaic)= (Dickinson) = (NIC)
Write:	<<HNM NNNN>>
Object:	G (SIMBAD class: Galaxy)
Note:	HST NICMOS maps of the entire HDFN. Galaxies from a list of Dickinson+, not published.
in source:	NAME HDFN
Ref:	=2001ApJ...559..620P
by	PAPOVICH C. , DICKINSON M., FERGUSON H.C.
	Astrophys. J., 559, 620-653 (2001)
	The stellar populations and evolution of Lyman break galaxies.
o	Table 2: <HNM NNNN> N=33 among (Nos 67-1541).
Ref:	=2003AJ....126.1183C
by	CONSELICE C.J. , BERSHADY M.A., DICKINSON M., PAPOVICH C.
	Astron. J., 126, 1183-1207 (2003)
	A direct measurement of major galaxy mergers at z≲3.
o	Table 3: <HNM NNNN> N=37 added among (Nos 40-1652).
Ref:	=2004AJ....127..131S
by	STANFORD S.A. , DICKINSON M., POSTMAN M., FERGUSON H.C., LUCAS R.A., CONSELICE C.J., BUDAVARI T., SOMERVILLE R.
	Astron. J., 127, 131-155 (2004)
	The evolution of early-type field galaxies selected from a NICMOS map of the Hubble Deep Field North.
o	Table 1: <HNM NNNN> N=160 added among (Nos 32-1594).
Ref:	=2004AJ....128..163L
by	LOTZ J.M. , PRIMACK J., MADAU P.
	Astron. J., 128, 163-182 (2004)
	A new nonparametric approach to galaxy morphological classification.
o	Table 7 <HNM NNNN> N=27 added among (Nos 72-1541).
=E=	Catalogue in electronic form as J/AJ/127/131
=E=	Catalogue in electronic form as J/AJ/128/163
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HNP2000]
[HNP2000]	(Harris+Nulsen+Ponman+, 2000) (Not yet in Simbad)
Write:	<<[HNP2000] 3C 295 WW>>
N:	2
Object:	Hot Spot (SIMBAD class: Radio = Radio Source)
Note:	Chandra X-ray detection of N=2 hot spots in 3C 295.
in source:	3C 295
Ref:	=2000ApJ...530L..81H
by	HARRIS D.E. , NULSEN P.E.J., PONMAN T.J., BAUTZ M., CAMERON R.A., DAVID L.P., DONNELLY R.H., FORMAN W.R., GREGO L., HARDCASTLE M.J., HENRY J.P., JONES C., LEAHY J.P., MARKEVITCH M., MARTEL A.R., McNAMARA B.R., MAZZOTTA P., TUCKER W., VIRANI S.N., VRTILEK J.
	Astrophys. J., 530, 81-84 (2000)
	Chandra X-ray detection of the radio hot spots of 3C 295.
o	p. L82 : PKS 0637-72 not identified. p. L83 : Spot B in 3C 390.3 = [D81b] 3C 390.3 B
o	Tables: <[HNP2000] 3C 295 WW> (Nos NW, SE).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HNP96]
[HNP96]	(Heidt+Nilsson+Pursimo+, 1996)
Write:	<<[HNP96] PKS 0139-097 A>>
N:	5
Object:	Feature (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Features towards the BL Lac object PKS 0139-097.
in source:	PKS 0139-097
Ref:	=1996A&A...312L..13H
by	HEIDT J. , NILSSON K., PURSIMO T., TAKALO L.O., SILLANPAA A.
	Astron. Astrophys., 312, 13-16 (1996)
	Possible absorbing systems towards the BL Lacertae object PKS 0139-097.
o	Table 1, Fig.1: <[HNP96] PKS 0139-097 A> (Nos A-D).
Ref:	=1999ApJ...521..134S
by	SCARPA R. , URRY C.M., FALOMO R., PESCE J.E., WEBSTER R., O'DOWD M., TREVES A.
	Astrophys. J., 521, 134-144 (1999)
	The Hubble space telescope survey of BL Lacertae objects: gravitational lens candidates and other unusual sources.
o	Fig.1: <[SUF99] 1ES OO33+595 A> (Nos A-B, G). Fig.6: <[SUF99] 1ES 1440+122 A> (Nos A-B, G). Fig.9: <[HNP96] PKS 0139-097 A> (No. E) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HNR99]
[HNR99]	(Holden+Nichol+Romer+, 1999)
Write:	<<[HNR99] PDCS NN NNN>>
N:	84
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	N=84 galaxies in 16 PDCS ClG. In the format the digits 'NNN' stand for the ID number assigned to each galaxy in the mask (ARC mask: numbering 'N', KPNO mask: numbering 'NNN' with always 3 digits).
Ref:	=1999AJ....118.2002H
by	HOLDEN B.P. , NICHOL R.C., ROMER A.K., METEVIER A., POSTMAN M., ULMER M.P., LUBIN L.M.
	Astron. J., 118, 2002-2013 (1999)
	Spectroscopic observations of optically selected clusters of galaxies from the Palomar distant cluster survey.
o	Table 2: <[HNR99] PDCS NN NNN> N=84.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HNS2000]
[HNS2000]	(Hearty+Neuhauser+Stelzer+, 2000)
Write:	<<[HNS2000] NN>> <<[HNS2000] NNa>>
N:	77+4
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC and ROSAT RASS observations. (Nos 1-77), X-ray sources found in the field of MBM 12. (Nos 49a-49b, 51a-51b) are possible optical counterparts of sources 49 and 51.
in source:	MBM 12
Ref:	=2000A&A...353.1044H
by	HEARTY T. , NEUHAEUSER R., STELZER B., FERNANDEZ M., ALCALA J.M., COVINO E., HAMBARYAN V.
	Astron. Astrophys., 353, 1044-1054 (2000)
	ROSAT PSPC observations of T Tauri stars in MBM 12.
o	Table 4: <[HNS2000] NN> (Nos 1-77), <[HNS2000] NNa> (Nos 49a-49b, 51a-51b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HNS99]
[HNS99]	(Heidt+Nilsson+Sillanpaa+, 1999) (Not yet in Simbad)
Write:	<<[HNS99] 1ES HHMM+DDd A>>
N:	23+4
Object:	G + * (SIMBAD class: Galaxy)
Note:	Figs 1, 2: N=23 host galaxies and galaxies in the field of N=7 '1ES' BL Lac objects. N=4 Stars 'S' in the same fields.
Ref:	=1999A&A...341..683H
by	HEIDT J. , NILSSON K., SILLANPAEAE A., TAKALO L.O., PURSIMO T.
	Astron. Astrophys., 341, 683-692 (1999)
	High-resolution imaging of Einstein Slew Survey BL Lacertae objects.
o	Figs 1, 2: <[HNS99] 1ES HHMM+DDd A> N=23, <[HNS99] 1ES HHMM+DDd S> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HNT
HNT	(Heydari-Malayeri+Niemela+Testor)
Write:	<<HNT Cluster>> <<HNT Star NN>>
N:	1+48
Object:	* (SIMBAD class: Star)
Note:	Table 4: N=1 Cl*, format 'Cluster', found in the literature as 'HNT 1'. N=48 stars in LHA 120-N 11C and 11D. See also [HRR2000].
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1987A&A...184..300H
by	HEYDARI-MALAYERI M. , NIEMELA V.S., TESTOR G.
	Astron. Astrophys., 184, 300-314 (1987)
	The LMC HII regions N 11C and E and their stellar contents.
o	'HNT Cluster' is found in literature as 'HNT 1'
o	Table 4: <HNT Cluster> N=1, <HNT Star NN> (Nos 1-48)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Ho
Ho	(Hogg)
*****	Avoid the usage of Ho, prefer Hogg
Details on Acronym: Ho
Ho	(Holmberg)
*****	Avoid the usage of Ho, prefer [H37]
Origin	of the Acronym: L (1982ApJS...50..319T)
Details on Acronym: Ho
Ho	(Holmberg)
*****	Avoid the usage of Ho, prefer [H37]
Origin	of the Acronym: L (1982ApJS...50..319T)
Details on Acronym: Ho
Ho	(Hodge)
*****	Avoid the usage of Ho, prefer [H69]
Origin	of the Acronym: L (1999PASP..111.1382O)
Details on Acronym: Ho
Ho	(Hodge)
*****	Avoid the usage of Ho, prefer [H77]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HO
HO	(Haggkvist+Oja)
*****	Avoid the usage of HO, prefer [HO73]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Ho
Ho	(Holmberg)
*****	Avoid the usage of Ho, prefer Holmberg
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HO2
HO2	(Hodge, Table 2)
*****	Avoid the usage of HO2, prefer [H81]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HO73]
[HO73]	(Haggkvist+Oja, 1973)= (HO) = (H.O.)
Write:	<<[HO73] +DD A>>
N:	96
Object:	* (SIMBAD class: Star)
Note:	Non-BD stars are designated by zone numbers (+8deg to +46deg) and letters. Identif. charts and 1855 coordinates
in source:	NAME NGP
Ref:	=1973A&AS...12..381H
by	HAGGKVIST L. , OJA T.
	Astron. Astrophys., Suppl. Ser., 12, 381-405 (1973)
	Photoelectric photometry of stars near the North Galactic Pole.
o	<[HO73] +DD A> N=96
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HO93]
[HO93]	(Hill+Oegerle, 1993)
Write:	<<[HO93] N-NNN>>
N:	611
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Format 'N-NNN': The first digit 'N-' is the table number, 'NNN' is a running number in each table, always a 3 digits number, beginning by the number 201. Table 3: 3-NNN, G in ACO 193, (Nos among 201-380). Table 4: 4-NNN, G in ACO 399 and ACO 401, (Nos among 201-619). Table 5: 5-NNN, G in ACO 1795, (Nos among 201-371). Table 6: 6-NNN, G in ACO 1809, (Nos among 201-326). Table 7: 7-NNN, G in ACO 2063, (Nos among 201-580). Table 8: 8-NNN, G in ACO 2124, (Nos among 201-347). See also [HO98]
in source:	ACO 193
in source:	ACO 399
in source:	ACO 401
in source:	ACO 1795
in source:	ACO 1809
in source:	ACO 2063
in source:	ACO 2124
Ref:	=1993AJ....106..831H
by	HILL J.M. , OEGERLE W.R.
	Astron. J., 106, 831-847 (1993)
	Dynamics of cD clusters of galaxies. I. Redshift data for seven clusters.
o	Table 3: <[HO93] 3-NNN> (Nos among 201-380). Table 4: <[HO93] 4-NNN> (Nos among 201-619). Table 5: <[HO93] 5-NNN> (Nos among 201-371). Table 6: <[HO93] 6-NNN> (Nos among 201-326). Table 7: <[HO93] 7-NNN> (Nos among 201-580). Table 8: <[HO93] 8-NNN> (Nos among 201-347). N=611
=E=	Catalogue in electronic form as J/AJ/106/831
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HO98]
[HO98]	(Hill+Oegerle, 1998)
Write:	<<[HO98] ACO NNNN NNN>>
N:	762
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Table 2: 'ACO 779 NNN', N=81 among (Nos 201-447). Table 3: 'ACO 1691 NNN', N=80 among (Nos 201-352). Table 4: 'ACO 1749 NNN', N=67 among (Nos 201-346). Table 5: 'ACO 1767 NNN', N=61 among (Nos 201-345). Table 6: 'ACO 1837 NNN', N=47 among (Nos 201-468). Table 7: 'ACO 1927 NNN', N=65 among (Nos 201-332). Table 8: 'ACO 2067 NNN', N=85 among (Nos 201-404). Table 9: 'ACO 2079 NNN', N=75 among (Nos 201-363). Table 10: 'ACO 2089 NNN', N=61 among (Nos 201-350). Table 11: 'ACO 2199 NNN', N=98 among (Nos 201-446). Table 12: 'ACO 2666 NNN', N=42 among (Nos 201-363). See also [HO93]
in source:	ACO 779
in source:	ACO 1691
in source:	ACO 1749
in source:	ACO 1767
in source:	ACO 1837
in source:	ACO 1927
in source:	ACO 2067
in source:	ACO 2079
in source:	ACO 2089
in source:	ACO 2199
in source:	ACO 2666
Ref:	=1998AJ....116.1529H
by	HILL J.M. , OEGERLE W.R.
	Astron. J., 116, 1529-1540 (1998)
	Dynamics of cD clusters of galaxies. III. Redshift data for 11 Abell clusters.
o	Tables 2-12: <[HO98] ACO NNNN NNN> N=762.
=E=	Catalogue in electronic form as J/AJ/116/1529
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Hoag
Hoag	(Hoag+)
*****	Avoid the usage of Hoag, prefer [HS77]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Hoag
Hoag	(Discoverer's name)
Write:	<<NAME Hoag N>>
N:	3
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	QSOs near M 82. Also [BJK80] 1, 2, 3
Ref:	=1980ApJ...242L..55B
by	BURBIDGE E.M. , JUNKKARINEN V.T., KOSKI A.T., SMITH H.E., HOAG A.A.
	Astrophys. J., 242, 55-57 (1980)
	A "cluster" of Quasi-Stellar Objects near M 82.
o	<NAME HOAG N> = <[BJK80] N> (Nos 1-3)
Details on Acronym: HOBYS
HOBYS	(Herschel imaging survey of OB Young Stellar Objects)
Write:	<<HOBYS JHHMMSS.s+DDMMSS>>
N:	46+177+23
Object:	(FIR) (SIMBAD class: FarIR = Far-IR source (λ >= 30 µm))
Note:	Herschel PACS and SPIRE observations, as part of the Herschel imaging survey of OB young stellar objects (HOBYS). For more information, visit: http://www.herschel.fr/cea/hobys/en/index.php
in source:	NGC 6334
in source:	NAME Mon R2 GMC
in source:	NGC 6357
Ref:	=2017A&A...602A..77T
by	TIGE J. , MOTTE F., RUSSEIL D., ZAVAGNO A., HENNEMANN M., SCHNEIDER N., HILL T., NGUYEN LUONG Q., DI FRANCESCO J., BONTEMPS S., LOUVET F., DIDELON P., KONYVES V., ANDRE P., LEULEU G., BARDAGI J., ANDERSON L.D., ARZOUMANIAN D., BENEDETTINI M., BERNARD J.-P., ELIA D., FIGUEIRA M., KIRK J., MARTIN P.G., MINIER V., MOLINARI S., NONY T., PERSI P., PEZZUTO S., POLYCHRONI D., RAYNER T., RIVERA-INGRAHAM A., ROUSSEL H., RYGL K., SPINOGLIO L., WHITE G.J.
	Astron. Astrophys., 602A, 77-77 (2017)
	The earliest phases of high-mass star formation, as seen in NGC 6334 by Herschel-HOBYS.
o	Table A.1: <HOBYS JHHMMSS.s+DDMMSS> N=46.
Ref:	=2017A&A...607A..22R
by	RAYNER T.S.M. , GRIFFIN M.J., SCHNEIDER N., MOTTE F., KONYVES V., ANDRE P., DI FRANCESCO J., DIDELON P., PATTLE K., WARD-THOMPSON D., ANDERSON L.D., BENEDETTINI M., BERNARD J.-P., BONTEMPS S., ELIA D., FUENTE A., HENNEMANN M., HILL T., KIRK J., MARSH K., MEN'SHCHIKOV A., NGUYEN LUONG Q., PERETTO N., PEZZUTO S., RIVERA-INGRAHAM A., ROY A., RYGL K., SANCHEZ-MONGE A., SPINOGLIO L., TIGE J., TREVINO-MORALES S.P., WHITE G.J.
	Astron. Astrophys., 607A, 22-22 (2017)
	Far-infrared observations of a massive cluster forming in the Monoceros R2 filament hub.
o	Table D.1: <HOBYS JHHMMSS.s+DDMMSS> N=177.
Ref:	=2019A&A...625A.134R
by	RUSSEIL D. , FIGUEIRA M., ZAVAGNO A., MOTTE F., SCHNEIDER N., MEN'SHCHIKOV A., BONTEMPS S., ANDRE P., ANDERSON L.D., BENEDETTINI M., DIDELON P., DI FRANCESCO J., ELIA D., KONYVES V., NGUYEN LUONG Q., NONY T., PEZZUTO S., RYGL K.L.J., SCHISANO E., SPINOGLIO L., TIGE J., WHITE G.J.
	Astron. Astrophys., 625A, 134-134 (2019)
	Herschel-HOBYS study of the earliest phases of high-mass star formation in NGC 6357.
o	Fig. D.1, Tables 4+C.2-C.4: <HOBYS JHHMMSS.s+DDMMSS> N=23. Table C.1: <[RFZ2019] NNN> (Nos 1-155). Table C.1, col(MDC): <[RFZ2019] MDC NN> (Nos 1-23).
=E=	Catalogue in electronic form as <J/A+A/602/A77/>
=E=	Catalogue in electronic form as <J/A+A/607/A22/>
=E=	Catalogue in electronic form as <J/A+A/625/A134/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HOD07
HOD07	(Hodapp, 2007)
Write:	<<HOD07 RNN>>
N:	27
Object:	RfN (SIMBAD class: RefNeb = Reflection Nebula)
Stat:	is completely incorporated in Simbad
Note:	UKIRT WFCAM NIR observations of the Mon R2 region: N=27 reflexion nebulae.
in source:	NAME Mon R2 GMC
Ref:	=2007AJ....134.2020H
by	HODAPP K.W.
	Astron. J., 134, 2020-2034 (2007)
	New H_{2} jets in Monoceros R2.
o	Table 2, col(3): <HOD07 RNN> (Nos R1-R27).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Hodge
Hodge	(Hodge)
*****	Avoid the usage of Hodge, prefer [H60b]
Details on Acronym: Hodge
Hodge	(Hodge)
*****	Avoid the usage of Hodge, prefer [H69]
Origin	of the Acronym: L (1980MNRAS.193..219P)
Details on Acronym: Hodge
Hodge	(Hodge)
*****	Avoid the usage of Hodge, prefer [H77]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Hodge
Hodge	(Hodge)
*****	Avoid the usage of Hodge, prefer H88
Origin	of the Acronym: L (1997ApJS..112..457W)
Details on Acronym: Hodge
Hodge	(Hodge)
*****	Avoid the usage of Hodge, prefer SMC Ass
Origin	of the Acronym: L (2000AJ....119.2214M)
Details on Acronym: Hodge-OB
Hodge-OB	(Hodge)
*****	Avoid the usage of Hodge-OB, prefer [H77]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HodgeC60
HodgeC60	(Hodge, Cluster, 1960)
*****	Avoid the usage of HodgeC60, prefer [H60b]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: HodgeC86
HodgeC86	(Hodge, Cluster, 1986)
*****	Avoid the usage of HodgeC86, prefer [H86]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: Hoff
Hoff	(Hoffmann+)
*****	Avoid the usage of Hoff, prefer HFE
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Hoffleit
Hoffleit	(Hoffleit)
*****	Avoid the usage of Hoffleit, prefer [H53]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: Hoffleit
Hoffleit	(Hoffleit)
*****	Avoid the usage of Hoffleit, prefer Hf
Details on Acronym: [HOG2000]
[HOG2000]	(Hunter+O'Connell+Gallagher+, 2000)
Write:	<<[HOG2000] NN>>
N:	48
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST images of NGC 1569. In addition to the 2 super-star clusters ([W91] A and B), the authors identify 45 other clusters and one association (No. 48).
in source:	NGC 1569
Ref:	=2000AJ....120.2383H
by	HUNTER D.A. , O'CONNELL R.W., GALLAGHER J.S., SMECKER-HANE T.A.
	Astron. J., 120, 2383-2401 (2000)
	The star clusters in the starburst irregular galaxy NGC 1569.
o	Table 2: <[HOG2000] NN> (Nos 1-48).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HOG2016]
[HOG2016]	(Holden+Oesch+Gonzalez+, 2016)
Write:	<<[HOG2016] BsNNNNNN>> <<[HOG2016] BNNNNN>>
N:	15+3
Object:	LBG (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	Keck I MOSFIRE spectroscopy of N=15+3 Lyman break galaxies (LBGs) in the GOODS-South field. Use of GOODS HST ACS and CANDELS data.
in source:	NAME GOODS-South Field
Ref:	=2016ApJ...820...73H
by	HOLDEN B.P. , OESCH P.A., GONZALEZ V.G., ILLINGWORTH G.D., LABBE I., BOUWENS R., FRANX M., VAN DOKKUM P., SPITLER L.
	Astrophys. J., 820, 73 (2016)
	Rest-frame optical emission lines in z ~ 3.5 lyman-break-selected galaxies: the ubiquity of unusually high [OIII]/Hβ ratios at 2 gyr.
o	Figs 1-3, Tables 1-3: <[HOG2016] BsNNNNNN> N=15 among (Nos Bs006507-Bs017524), <[HOG2016] BNNNNN> N=3 among (Nos B14623-B17453).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HOG94]
[HOG94]	(Hunter+O'Connell+Gallagher, 1994)
Write:	<<[HOG94] NN>>
N:	14
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	All objects are Cl*, except [HOG94] 5 'more difffuse than the others'
in source:	NGC 1140
Ref:	=1994AJ....108...84H
by	HUNTER D.A. , O'CONNELL R.W., GALLAGHER III J.S.
	Astron. J., 108, 84-89 (1994)
	Hubble Space Telescope imaging of the central star-forming region in NGC 1140.
o	Table 2: <[HOG94] NN> N=14
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HOG96]
[HOG96]	(Hall+Osmer+Green+, 1996)= (DMS) = (N)
Write:	<<[HOG96] DMS HHMM+DDMM>> <<[HOG96] DMS HHMM.m+DDMM>> <<[HOG96] DMS NN>> <<[HOG96] NHHMM+DDMM>> <<[HOG96] NHHMM.m+DDMM>> <<[HOG96] N NN>>
N:	21375
Object:	Poss. QSO + QSO + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	QSO candidates or QSO, format 'DMS HHMM+DDMM' or 'DMS HHMM.m+DDMM', where DMS stands for Deep Multicolor Survey. This format is cross-id. with the format 'DMS NN' (Nos 1-55). Galaxies, format 'AHHMM+DDMM' or 'AHHMM.m+DDMM' where the letter 'A' stands for 'N' (Narrow em.-line galaxy). This format is cross-id. with the format 'A NN' (Nos 1-43)
Ref:	=1996ApJ...462..614H
by	HALL P.B. , OSMER P.S., GREEN R.F., PORTER A.C., WARREN S.J.
	Astrophys. J., 462, 614-636 (1996)
	A deep multicolor survey. II. Initial spectroscopy and comparison with expected quasar number counts.
o	(Erratum) 1996ApJ...471.1073H
o	Table 1: <[HOG96] DMS HHMM+DDMM>, <[HOG96] DMS HHMM.m+DDMM> = <[HOG96] DMS NN> (Nos 1-46). Table 2: <[HOG96] NHHMM+DDMM>, <[HOG96] NHHMM.m+DDMM> = <[HOG96] N NN> (Nos N 1 to N 39).
Ref:	=1997AJ....114.2269K
by	KENNEFICK J.D. , OSMER P.S., HALL P.B., GREEN R.F.
	Astron. J., 114, 2269-2275 (1997)
	A deep multicolor survey. III. Additional spectroscopy and implications for the number counts of faint quasars.
o	Table 1: <[HOG96] DMS HHMM+DDMM> = <[HOG96] DMS NN> N=9 (Nos 47-55). Table 2: <[HOG96] NHHMM+DDMM> = <[HOG96] N NN> N=4 (Nos N 40 to N 43).
=E=	Catalogue in electronic form as J/ApJ/462/614
=E=	Catalogue in electronic form as J/AJ/114/2269
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Hogg
Hogg	(Hogg)= (Ho)
Write:	<<Cl Hogg NNN>>
N:	133
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Ref:	=1965MmMtS..17....1H
by	HOGG A.R.
	Mem. Mount Stromlo Obs., 17, 1-17 (1965)
	Catalogue of open clusters south of -45° declination.
o	Catalogue: <Cl Hogg NNN> (Nos 1-133)
Details on Acronym: [HOJ2002]
[HOJ2002]	(Hansen+Olsen+Jorgensen, 2002)
Write:	<<[HOJ2002] EIS JHHMM+DDMM NN>>
N:	38+18+37+12+19
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Observations from the Danish 1.5 m telescope at ESO. Spectroscopy of 5 EIS clusters. See also [OHJ2003].
in source:	[SOD99] EIS J0946-2029
in source:	[SOD99] EIS J0947-2120
in source:	[SOD99] EIS J0948-2044
in source:	[SOD99] EIS J0949-2101
in source:	[SOD99] EIS J0956-2059
Ref:	=2002A&A...388....1H
by	HANSEN L. , OLSEN L.F., JORGENSEN H.E.
	Astron. Astrophys., 388, 1-6 (2002)
	Multi-object spectroscopy of low redshift EIS clusters. I.
o	Table A1: <[HOJ2002] EIS J0946-2029 NN> (Nos 1-38). Table A2: <[HOJ2002] EIS J0947-2120 NN> (Nos 1-18). Table A3: <[HOJ2002] EIS J0948-2044 NN> (Nos 1-37). Table A4: <[HOJ2002] EIS J0949-2101 NN> (Nos 1-12). Table A5: <[HOJ2002] EIS J0956-2059 NN> (Nos 1-19).
=E=	Catalogue in electronic form as J/A+A/388/1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HOK2009]
[HOK2009]	(Hatch+Overzier+Kurk+, 2009)
Write:	<<[HOK2009] NN>>
N:	21
Object:	G (SIMBAD class: Galaxy)
Note:	HST ACS and VLT SINFONI observations of the protocluster surrounding MRC 1138-262. See also [KPR2004].
in source:	NAME Spiderweb protocluster = NAME MRC 1138-262 Protocluster
Ref:	=2009MNRAS.395..114H
by	HATCH N.A. , OVERZIER R.A., KURK J.D., MILEY G.K., ROTTGERING H.J.A., ZIRM A.W.
	Mon. Not. R. Astron. Soc., 395, 114-125 (2009)
	The growth and assembly of a massive galaxy at z ~ 2.
o	Table 1, Fig. 2-3: <[HOK2009] NN> (Nos 1-19).
Ref:	=2011MNRAS.415.2245K
by	KUIPER E. , HATCH N.A., MILEY G.K., NESVADBA N.P.H., ROTTGERING H.J.A., KURK J.D., LEHNERT M.D., OVERZIER R.A., PENTERICCI L., SCHAYE J., VENEMANS B.P.
	Mon. Not. R. Astron. Soc., 415, 2245-2256 (2011)
	A SINFONI view of flies in the Spiderweb: a galaxy cluster in the making.
o	Fig. 2, Table 2: <[HOK2009] NN> (Nos 20-21) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Hole
Hole	(Hole)
*****	Avoid the usage of Hole, prefer [WM98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Holm
Holm	(Holmberg, 1937) (Not yet in Simbad)
*****	Avoid the usage of Holm, prefer [H37]
Origin	of the Acronym: L (2011ApJ...728..124R)
Details on Acronym: Holm
Holm	(Holmberg) (Not yet in Simbad)
*****	Avoid the usage of Holm, prefer [H37]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Holm
Holm	(Holmberg)
*****	Avoid the usage of Holm, prefer Holmberg
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Holmberg
Holmberg	(Holmberg, 1937) (Not yet in Simbad)
*****	Avoid the usage of Holmberg, prefer [H37]
Origin	of the Acronym: L (2011ApJ...728..124R)
Details on Acronym: Holmberg
Holmberg	(Holmberg) (Not yet in Simbad)
*****	Avoid the usage of Holmberg, prefer [H37]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Holmberg
Holmberg	(Holmberg)= (Ho) = (Holm)
Write:	<<Holmberg R>>
N:	9
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Holmberg I, II, III are in M 81 region. Holmberg IV, V are in M 101 region. Holmberg IX is found later in the literature
Ref:	=1950MeLu2.128....1H
by	HOLMBERG E.
	Lund Medd. Astron. Obs. Ser. II, 128, 1-None (1950)
	A photometric study of nearby galaxies.
o	<Holmberg R> (Nos I-V)
Ref:	=1958MeLu2.136....1H
by	HOLMBERG E.
	Lund Medd. Astron. Obs. Ser. II, 136, 1-None (1958)
	A photographic photometry of extragalactic nebulae.
o	<Holmberg R> (Nos VI-VIII)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Holtz
Holtz	(Holtzman+) (Not yet in Simbad)
*****	Avoid the usage of Holtz, prefer [HWM96]
Origin	of the Acronym: L (2000MNRAS.312..703F)
Details on Acronym: [HOM84]
[HOM84]	(Halpern+Marshall+Oke, 1984)
Write:	<<[HOM84] 1300+361 A>>
N:	2
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	5-m Hale telescope spectroscopy.
Ref:	=1984AJ.....89.1802H
by	HALPERN J.P. , MARSHALL H.L., OKE J.B.
	Astron. J., 89, 1802-1807 (1984)
	1300+361 A, B is not a gravitational lens.
o	<[HOM84] 1300+361 A> (Nos A, B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HOO2016]
[HOO2016]	(Harikane+Ouchi+Ono+, 2016)
Write:	<<[HOO2016] zN-aeg-NNNNN>> <<[HOO2016] zN-uds-NNNNN>> <<[HOO2016] zN-cos-NNNNN>> <<[HOO2016] zN-gdnw-NNNNN>> <<[HOO2016] zN-gdnd-NNNNN>> <<[HOO2016] zN-gdsw-NNNNN>> <<[HOO2016] zN-gdsd-NNNNN>> <<[HOO2016] zN-xdf-NNNN>> <<[HOO2016] zN-m0416p-NNNN>> <<[HOO2016] zN-a2744p-NNNN>>
N:	9651
Object:	LBG (SIMBAD class: Galaxy)
Note:	N=9651 Lyman break galaxies (LBGs) at z∼4-7 identified in the Hubble legacy deep imaging data, in the following fields: CANDELS-AEGIS ("aeg"), CANDELS-COSMOS ("cos"), CANDELS-UDS ("uds"), GOODS-North (Deep and Wide, "gdnd" and "gdnw"), GOODS-South (Deep and Wide, "gdsd" and "gdsw"), Hubble Ultra Deep Field (HUDF, "xdf"), and two Hubble Frontier Fields HFF-parallel (HFF-Abell2744P and HFF-MACS0416P, "a2744p" and "m0416p").
in source:	NAME Extended Groth Strip
in source:	NAME COSMOS Field
in source:	NAME GOODS North Field
in source:	NAME GOODS South Field
in source:	NAME HUDF
Ref:	=2016ApJ...821..123H
by	HARIKANE Y. , OUCHI M., ONO Y., MORE S., SAITO S., LIN Y.-T., COUPON J., SHIMASAKU K., SHIBUYA T., PRICE P.A., LIN L., HSIEH B.-C., ISHIGAKI M., KOMIYAMA Y., SILVERMAN J., TAKATA T., TAMAZAWA H., TOSHIKAWA J.
	Astrophys. J., 821, 123-123 (2016)
	Evolution of stellar-to-halo mass ratio at z = 0 - 7 identified by clustering analysis with the Hubble legacy imaging and early Subaru/Hyper Suprime-Cam survey data.
o	Table 3: <[HOO2016] zN-aeg-NNNNN> N=510 among (Nos z5-aeg-180 to z7-aeg-35824), <[HOO2016] zN-uds-NNNNN> N=400 among (Nos z5-uds-736 to z7-uds-23944), <[HOO2016] zN-cos-NNNNN> N=455 among (Nos z5-cos-108 to z7-cos-26205), <[HOO2016] zN-gdnw-NNNNN> N=1123 among (Nos z4-gdnw-31 to z7-gdnw-36823), <[HOO2016] zN-gdnd-NNNNN> N=2534 among (Nos z4-gdnd-3144 to z7-gdnd-38101), <[HOO2016] zN-gdsw-NNNNN> N=734 among (Nos z4-gdsw-484 to z7-gdsw-13271), <[HOO2016] zN-gdsd-NNNNN> N=3082 among (Nos z4-gdsd-7260 to z7-gdsd-44989), <[HOO2016] zN-xdf-NNNN> N=614 among (Nos z4-xdf-780 to z7-xdf-5942), <[HOO2016] zN-m0416p-NNNN> N=129 among (Nos z5-m0416p-166 to z7-m0416p-3210), <[HOO2016] zN-a2744p-NNNN> N=70 among (Nos z5-a2744p-325 to z7-a2744p-2647).
=E=	Catalogue in electronic form as <J/ApJ/821/123/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HOO2019]
[HOO2019]	(Higuchi+Ouchi+Ono+, 2019)= ([HOO2019a])
Write:	<<[HOO2019] HSC-z6PCCNN>> <<[HOO2019] HSC-z7PCCNN>>
N:	14+26
Object:	Poss. Protocluster (SIMBAD class: ClG_Candidate = Cluster of Galaxies Candidate)
Stat:	is completely incorporated in Simbad
Note:	Keck DEIMOS and Magellan-I Baade Telescope IMACS observations of N=14+26 protocluster candidates at z=5.7 and z=6.6 respectively. Use of Subaru/Hyper Suprime-Cam (HSC) deep images, and also Keck, Subaru, and Magellan spectra, and literature data.
Ref:	=2019ApJ...879...28H
by	HIGUCHI R. , OUCHI M., ONO Y., SHIBUYA T., TOSHIKAWA J., HARIKANE Y., KOJIMA T., CHIANG Y.-K., EGAMI E., KASHIKAWA N., OVERZIER R., KONNO A., INOUE A.K., HASEGAWA K., FUJIMOTO S., GOTO T., ISHIKAWA S., ITO K., KOMIYAMA Y., TANAKA M.
	Astrophys. J., 879, 28-28 (2019)
	SILVERRUSH. VII. Subaru/HSC identifications of protocluster candidates at z ~ 6-7: implications for cosmic reionization.
o	Table 4: <[HOO2019] HSC-z6PCCNN> (Nos PCC1-PCC14), <[HOO2019] HSC-z7PCCNN> (Nos PCC1-PCC26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HOO2019a]
[HOO2019a]	(Higuchi+Ouchi+Ono+, 2019)
*****	Avoid the usage of [HOO2019a], prefer [HOO2019]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HOO2019b]
[HOO2019b]	(Harikane+Ouchi+Ono+, 2019)
Write:	<<[HOO2019b] z57LAE-NN>> <<[HOO2019b] z66LAE-NN>>
N:	44+12
Object:	LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Gemini GMOS and Keck II DEIMOS observations of N=44+12 Lyman Alpha Emitters (LAEs) in two overdensities at z=5.692 (z57OD, [HOO2019] HSC-z6PCC1) and z=6.585 (z66OD, [HOO2019] HSC-z7PCC24) respectively.
in source:	[HOO2019] HSC-z6PCC1
in source:	[HOO2019] HSC-z7PCC24
Ref:	=2019ApJ...883..142H
by	HARIKANE Y. , OUCHI M., ONO Y., FUJIMOTO S., DONEVSKI D., SHIBUYA T., FAISST A.L., GOTO T., HATSUKADE B., KASHIKAWA N., KOHNO K., HASHIMOTO T., HIGUCHI R., INOUE A.K., LIN Y.-T., MARTIN C.L., OVERZIER R., SMAIL I., TOSHIKAWA J., UMEHATA H., AO Y., CHAPMAN S., CLEMENTS D.L., IM M., JING Y., KAWAGUCHI T., LEE C.-H., LEE M.M., LIN L., MATSUOKA Y., MARINELLO M., NAGAO T., ONODERA M., TOFT S., WANG W.-H.
	Astrophys. J., 883, 142-142 (2019)
	SILVERRUSH. VIII. Spectroscopic identifications of early large-scale structures with protoclusters over 200 Mpc at z ~ 6-7: strong associations of dusty star-forming galaxies.
o	Table 1: <[HOO2019b] z57LAE-NN> (Nos 1-44). Table 2: <[HOO2019b] z66LAE-NN> (Nos 1-12).
o	Table 3: Not all protoclusters are in SIMBAD.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HOO2023]
[HOO2023]	(Harikane+Ouchi+Oguri+, 2023)
Write:	<<[HOO2023] GL-z9-NN>> <<[HOO2023] SM-z12-1>> <<[HOO2023] GL-z12-1>> <<[HOO2023] CR2-z12-N>> <<[HOO2023] CR3-z12-1>> <<[HOO2023] S5-z12-1>> <<[HOO2023] CR2-z16-1>> <<[HOO2023] S5-z16-1>>
N:	23
Object:	Poss. G (SIMBAD class: Galaxy_Candidate = Galaxy Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=23 dropout galaxy candidates in five fields observed by the JWST (SMACS J0723.3-7327 SM, GLASS GL, CEERS2 CR2, Stephan's Quintet S5). Use of JWST archival data.
Ref:	=2023ApJS..265....5H
by	HARIKANE Y. , OUCHI M., OGURI M., ONO Y., NAKAJIMA K., ISOBE Y., UMEDA H., MAWATARI K., ZHANG Y.
	Astrophys. J., Suppl. Ser., 265, 5 (2023)
	A Comprehensive Study of Galaxies at z ~ 9-16 Found in the Early JWST Data: Ultraviolet Luminosity Functions and Cosmic Star Formation History at the Pre-reionization Epoch.
o	Table 3: <[HOO2023] GL-z9-N> (Nos 1-13). Table 4: <[HOO2023] SM-z12-1> N=1, <[HOO2023] GL-z12-1> N=1, <[HOO2023] CR2-z12-N> (Nos 1-4), <[HOO2023] CR3-z12-1> N=1, <[HOO2023] S5-z12-1> N=1. Table 5: <[HOO2023] CR2-z16-1> N=1, <[HOO2023] S5-z16-1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HOPS
HOPS	(Herschel Orion Protostar Survey)
Write:	<<HOPS NNN>>
Object:	Protostar (SIMBAD class: YSO = Young Stellar Object)
Note:	Herschel PACS photometry and spectroscopy within the Herschel Orion Protostar Survey. Only the first references citing HOPS sources are given here.
Ref:	=2010A&A...518L..94S
by	STANKE T. , STUTZ A.M., TOBIN J.J., ALI B., MEGEATH S.T., KRAUSE O., LINZ H., ALLEN L., BERGIN E., CALVET N., DI FRANCESCO J., FISCHER W.J., FURLAN E., HARTMANN L., HENNING T., MANOJ P., MARET S., MUZEROLLE J., MYERS P.C., NEUFELD D., OSORIO M., PONTOPPIDAN K., POTEET C.A., WATSON D.M., WILSON T.
	Astron. Astrophys., 518L, 94-94 (2010)
	Hier ist wahrhaftig ein Loch im Himmel. The NGC 1999 dark globule is not a globule.
o	Fig. 2, Fig. A.1: <HOPS NNN> (Nos 166, 168, 171, 203, 362). Fig. 3, Table B.1: <[SST2010] N> (Nos 1-5). Fig. 1-2, Fig. A.1: <NAME HH 147 IR>.
Ref:	=2010A&A...518L.122F
by	FISCHER W.J. , MEGEATH S.T., ALI B., TOBIN J.J., OSORIO M., ALLEN L.E., KRYUKOVA E., STANKE T., STUTZ A.M., BERGIN E., CALVET N., DI FRANCESCO J., FURLAN E., HARTMANN L., HENNING T., KRAUSE O., MANOJ P., MARET S., MUZEROLLE J., MYERS P., NEUFELD D., PONTOPPIDAN K., POTEET C.A., WATSON D.M., WILSON T.
	Astron. Astrophys., 518L, 122-122 (2010)
	Herschel-PACS imaging of protostars in the HH 1-2 outflow complex.
o	Table 1: <HOPS NNN> (No. 165) added.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Hornoch
Hornoch	(Hornoch)
Write:	<<Hornoch NN>>
N:	41
Object:	Nova (SIMBAD class: Nova = Classical Nova)
Note:	Photometry of Novae in the M31N catalogue by Kamil Hornoch.
in source:	M 31 = NGC 224
Ref:	=2007A&A...465..375P
by	PIETSCH W. , HABERL F., SALA G., STIELE H., HORNOCH K., RIFFESER A., FLIRI J., BENDER R., BUEHLER S., BURWITZ V., GREINER J., SEITZ S.
	Astron. Astrophys., 465, 375-392 (2007)
	X-ray monitoring of optical novae in M 31 from July 2004 to February 2005.
o	Paragraph 4.2 CXOM31 J004238.2+411000 is a misprint for CXOM31 J04228.2+411000
o	Table a1: <M31N YYYY-MMa> N=719. Table b2: <Hornoch NN> (Nos 1-41).
=E=	Catalogue in electronic form as J/A+A/465/375
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HOS2013]
[HOS2013]	(Hashimoto+Ouchi+Shimasaku+, 2013)
Write:	<<[HOS2013] CDFS-NNNN>> <<[HOS2013] COSMOS-NNNNN>>
N:	2+3
Object:	LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Magellan MMIRS and Keck II NIRSPEC spectroscopy of N=5 Lyα emitters at z∼2.2.
in source:	NAME CDFS
in source:	NAME COSMOS Field
Ref:	=2013ApJ...765...70H
by	HASHIMOTO T. , OUCHI M., SHIMASAKU K., ONO Y., NAKAJIMA K., RAUCH M., LEE J., OKAMURA S.
	Astrophys. J., 765, 70 (2013)
	Gas motion study of Lyα emitters at z ~ 2 using FUV and optical spectral lines.
o	(Erratum) erratum vol. 775, art. 140 (2013)
o	Table 1: <[HOS2013] CDFS-NNNN> (Nos 3865, 6482), <[HOS2013] COSMOS-NNNNN> (Nos 13636, 30679, 43982).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Houck
Houck	(Houck+)
*****	Avoid the usage of Houck, prefer [HSW2005]
Origin	of the Acronym: L (2008ApJ...680..119B)
Details on Acronym: HOY
HOY	(Herschel Orion YSO)
Write:	<<HOY JHHMMSS.ss+DDMMSS.s>>
N:	43
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	Herschel PACS 70 and 160micron observations of the Oriona Nebula Cluster.
in source:	NAME Orion Nebula Cluster
Ref:	=2012ApJ...753L..35B
by	BILLOT N. , MORALES-CALDERON M., STAUFFER J.R., MEGEATH S.T., WHITNEY B.
	Astrophys. J., 753L, 35 (2012)
	Herschel far-infrared photometric monitoring of protostars in the Orion Nebula Cluster.
o	Table 1: <HOY JHHMMSS.ss+DDMMSS.s> N=43
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HOY2015]
[HOY2015]	(Hatsukade+Ohta+Yabe+, 2015)
Write:	<<[HOY2015] ASN>>
N:	8
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 6 observations of N=8 1.3mm sources detected toward 6 galaxies from K-band selected source catalog of Yabe et al. (2012PASJ...64...60Y, see also [YOI2012]).
in source:	NAME SXDF
Ref:	=2015ApJ...810...91H
by	HATSUKADE B. , OHTA K., YABE K., SEKO A., MAKIYA R., AKIYAMA M.
	Astrophys. J., 810, 91 (2015)
	Optical-infrared properties of faint 1.3 mm sources detected with ALMA.
o	Fig. 1, Table 1: <[HOY2015] ASN> (Nos AS1-AS8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HP
HP	(Hayashi+Pyo) (Not yet in Simbad)
*****	Avoid the usage of HP, prefer [HP2009b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HP
HP	(Obs. de Haute Provence)
*****	Avoid the usage of HP, prefer Haute-Provence
Details on Acronym: HP
HP	(HII, Pellet)
*****	Avoid the usage of HP, prefer [PAV78]
Origin	of the Acronym: L (1980A&AS...40...67D)
Details on Acronym: HP
HP	(Harvard obs., Pulsar)
Rem:	Superseded by PSR
*****	Avoid the usage of HP, prefer PSR
Details on Acronym: [HP2001]
[HP2001]	(Haberl+Pietsch, 2001)
Write:	<<[HP2001] NNN>>
N:	184
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Archival ROSAT observations of M 33.
in source:	M 33 = NGC 598
Ref:	=2001A&A...373..438H
by	HABERL F. , PIETSCH W.
	Astron. Astrophys., 373, 438-446 (2001)
	The X-ray view of M 33 after ROSAT.
o	Table 2: <[HP2001] NNN> (Nos 1-184).
=E=	Catalogue in electronic form as J/A+A/373/438
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HP2004]
[HP2004]	(Haberl+Pietsch, 2004)
Write:	<<[HP2004] NN>>
Object:	X-ray Binary (SIMBAD class: HighMassXBin = High Mass X-ray Binary)
Note:	XMM-Newton observations of the SMC: 65 Be and X-ray binaries are found, (Nos 55-65) without X-ray coordinates listed due to their large uncertainties.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2004A&A...414..667H
by	HABERL F. , PIETSCH W.
	Astron. Astrophys., 414, 667-676 (2004)
	X-ray observations of Be/X-ray binaries in the SMC.
o	Table 3: <[HP2004] NN> (Nos 1-65).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HP2005]
[HP2005]	(Henkel+Partridge, 2005)
Write:	<<[HP2005] NN>>
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	NRAO VLA observations of very faint sources at 8.5GHz.
Ref:	=2005ApJ...635..950H
by	HENKEL B. , PARTRIDGE R.B.
	Astrophys. J., 635, 950-958 (2005)
	Completing the counts of radio sources at 8.5GHz.
o	Table 2: <[HP2005] NN> (Nos 1-47).
=E=	Catalogue in electronic form as J/ApJ/635/950
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HP2007]
[HP2007]	(Hidalgo-Gamez+Peimbert, 2007)= (DIG) (Not yet in Simbad)
Write:	<<[HP2007] DIG W>>
N:	3
Object:	Diffuse Ionized Gas (SIMBAD class: Cloud)
Note:	FORS1 VLT in Cerro Paranal observations of NGC 6822. Search for Diffuse Ionized Gas.
in source:	NGC 6822
Ref:	=2007AJ....133.1874H
by	HIDALGO-GAMEZ A.M. , PEIMBERT A.
	Astron. J., 133, 1874-1882 (2007)
	Diffuse ionized gas inside the dwarf irregular galaxy NGC 6822.
o	Fig.1, Table 1: <[HP2007] DIG W> (Nos E, C, W).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HP2009]
[HP2009]	(Hernandez-Martinez+Pena, 2009)= ([HP2009a])
Write:	<<[HP2009] PN NN>> <<[HP2009] HII NN>> <<[HP2009] Ha NN>>
N:	26+25+21
Object:	PN + HII + EmO (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	CTIO 4m Blanco telescope MOSAIC2 images and VLT FORS2 spectroscopy of NGC 6822.
in source:	NGC 6822
Ref:	=2009A&A...495..447H
by	HERNANDEZ-MARTINEZ L. , PENA M.
	Astron. Astrophys., 495, 447-455 (2009)
	Emission line objects in NGC6822. New planetary nebula candidates.
o	Table 2: <[HP2009] PN NN> (Nos 1-26), <[HP2009] HII NN> (Nos 1-25), <[HP2009] Ha NN> (Nos 1-21).
=E=	Catalogue in electronic form as J/A+A/495/447
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HP2009a]
[HP2009a]	(Hernandez-Martinez+Pena, 2009)
*****	Avoid the usage of [HP2009a], prefer [HP2009]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HP2009b]
[HP2009b]	(Hayashi+Pyo, 2009)= (HP) (Not yet in Simbad)
Write:	<<[HP2009b] N>> <<[HP2009b] NW>>
N:	7
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Subaru MOIRCS NIR observations of L1551 dark cloud.
in source:	LDN 1551
Ref:	=2009ApJ...694..582H
by	HAYASHI M. , PYO T.-S.
	Astrophys. J., 694, 582-592 (2009)
	Wide-field near-infrared imaging of the L1551 dark cloud.
o	Table 1: <[HP2009b] N> (Nos 1-6), <[HP2009b] NW> (No. 3E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HP80]
[HP80]	(Hawley+Phillips, 1980) (Not yet in Simbad)
Write:	<<[HP80] R>>
N:	9
Object:	HII (SIMBAD class: HIIReg = HII Region)
in source:	NGC 1566
Ref:	=1980ApJ...235..783H
by	HAWLEY S.A. , PHILLIPS M.M.
	Astrophys. J., 235, 783-792 (1980)
	Spectrophotometry of HII regions and the nucleus of NGC 1566.
o	Fig.1: <[HP80] R> (Nos I to IX).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HP86]
[HP86]	(Houck+Pollock, 1986)
Write:	<<[HP86] NN>>
N:	16
Object:	* (SIMBAD class: Star)
Note:	N=16 comparison stars in the field of AR Boo.
Ref:	=1986PASP...98..461H
by	HOUCK J.C. , POLLOCK J.T.
	Publ. Astron. Soc. Pac., 98, 461-463 (1986)
	The light curve of the eclipsing binary AR Bootis.
o	Table I: <[HP86] NN> (Nos 1-16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HP99]
[HP99]	(Haberl+Pietsch, 1999)
Write:	<<[HP99] NNNNN>>
N:	758
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Sub-sample of variable X-ray sources observed by ROSAT PSPC in the LMC. The complete list of LMC sources contains more than 60000 objects. See also ROSAT PSPC [HFP2000] in the SMC. See also ROSAT HRI in the LMC and SMC [SHP2000].
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1999A&A...344..521H
by	HABERL F. , PIETSCH W.
	Astron. Astrophys., 344, 521-532 (1999)
	Variable X-ray sources in the LMC region observed by the ROSAT PSPC.
o	Tables 1, 2: <[HP99] NNNN> N=758 among (Nos 61-1225).
Ref:	=1999A&AS..139..277H
by	HABERL F. , PIETSCH W.
	Astron. Astrophys., Suppl. Ser., 139, 277-295 (1999)
	A ROSAT PSPC catalogue of X-ray sources in the LMC region.
o	Table 1: <[HP99] NNNN> N=758 among (Nos 1-1367).
=E=	Catalogue in electronic form as J/A+A/344/521
=E=	Catalogue in electronic form as J/A+AS/139/277
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPA2000]
[HPA2000]	(Hogg+Pahre+Adelberger+, 2000)
Write:	<<[HPA2000] JHHMMSS.ss+DDMMSS.s>>
N:	3606+487+22
Object:	G (SIMBAD class: Galaxy)
Note:	Detection and photometry of sources in a region centered on the HDF. See also [CHB2000], [C2001b].
in source:	NAME HDFN
Ref:	=2000ApJS..127....1H
by	HOGG D.W. , PAHRE M.A., ADELBERGER K.L., BLANDFORD R., COHEN J.G., GAUTIER T.N., JARRETT T., NEUGEBAUER G., STEIDEL C.C.
	Astrophys. J., Suppl. Ser., 127, 1-9 (2000)
	Caltech faint galaxy redshift survey. IX. Source detection and photometry in the Hubble Deep Field region.
o	Tables 2-4: <[HPA2000] JHHMMSS.ss+DDMMSS.s> N=3606+487+22.
=E=	Catalogue in electronic form as J/ApJS/127/1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPC2015]
[HPC2015]	(Hennawi+Prochaska+Cantalupo+, 2015)
Write:	<<[HPC2015] SDSSJ0841+3921 nebula>> <<[HPC2015] SDSSJ0841+3921 protocluster>> <<[HPC2015] AGNN>> <<[HPC2015] JHHMMSS.sss+DDMMSS.ss>>
N:	1+1+3+61
Object:	Protocluster + AGN + Em. Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Keck-I LRIS narrow-band imaging and Keck-II DEIMOS spectroscopy of N=1 giant Lyman α nebula, N=1 protocluster, N=3 AGNs, and N=61 LAE candidates in the field of SDSS J084158.47+392121.0.
Ref:	=2015Sci...348..779H
by	HENNAWI J.F. , PROCHASKA J.X., CANTALUPO S., ARRIGONI-BATTAIA F.
	Sci, 348, 779-783 (2015)
	Quasar quartet embedded in giant nebula reveals rare massive structure in distant universe.
o	<[HPC2015] SDSSJ0841+3921 nebula> = <NAME Jackpot Nebula>. <[HPC2015] SDSSJ0841+3921 protocluster> N=1. Fig. 1, Table S1: <[HPC2015] AGNN> (Nos AGN1-AGN3). Table S4: <[HPC2015] JHHMMSS.sss+DDMMSS.ss> N=61.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HPD
HPD	(Hester+Parker+Dufour) (Not yet in Simbad)
*****	Avoid the usage of HPD, prefer [HPD83]
Origin	of the Acronym: L (1986ApJ...300..675H)
Details on Acronym: HPD
HPD	(Haug+Pfleiderer+Dachs)
Write:	<<HPD Nor NNN>> <<HPD Cir NN>>
N:	105+38
Object:	* (SIMBAD class: Star)
Note:	Table 1: format 'Nor NNN', N=105 stars in Norma. Table 2: format 'Cir NN', N=38 stars in Circinus
Ref:	=1966ZA.....64..140H
by	HAUG U. , PFLEIDERER J., DACHS J.
	Zeitschr. Astrophys., 64, 140-157 (1966)
	Sterne fruhen Spektraltyps in Norma und Circinus.
o	Table 1: <HPD Nor NNN> N=105, Table 2: <HPD Cir NN> N=38
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HPD2003]
[HPD2003]	(Herbig+Petrov+Duemmler, 2003) (Not yet in Simbad)
Write:	<<[HPD2003] V1057 Cyg A>>
N:	4
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Spectroscopy of V1057 Cyg. Features A, B, C are very near the star, C appears as a structural blob, A, B, D as Arcs.
Ref:	=2003ApJ...595..384H
by	HERBIG G.H. , PETROV P.P., DUEMMLER R.
	Astrophys. J., 595, 384-411 (2003)
	High-resolution spectroscopy of FU Orionis stars.
o	Fig.15: <[HPD2003] V1057 Cyg A> (Nos A-D).
Details on Acronym: [HPD2006]
[HPD2006]	(Herbert-Fort+Prochaska+Dessauges-Zavzdsky+, 2006)
Write:	<<[HPD2006] SDSS JHHMMSS.ss+DDMMSS.s abs N.NNN>>
N:	435
Object:	DLA
Note:	Search for strong DLAs in the SDSS QSOs.
Ref:	=2006PASP..118.1077H
by	HERBERT-FORT S. , PROCHASKA J.X., DESSAUGES-ZAVADSKY M., ELLISON S.L., HOWK J.C., WOLFE A.M., PROCHTER G.E.
	Publ. Astron. Soc. Pac., 118, 1077-1097 (2006)
	The metal-strong damped Lyα systems.
o	Paragr.1: FJ 0812+32 = QSO J0812+3208 in SIMBAD (confusion between 1950 and 2000 coordinates), and the DLA with z=2.626 is [PHW2003] Galaxy in SIMBAD.
o	Table 3: <[HPD2006] SDSS JHHMMSS.ss+DDMMSS.s abs N.NNN> N=435.
=E=	Catalogue in electronic form as J/PASP/118/1077
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPD83]
[HPD83]	(Hester+Parker+Dufour, 1983)= (HPD) (Not yet in Simbad)
Write:	<<[HPD83] Star A>> <<[HPD83] Region R>> <<[HPD83] Spur>>
N:	3+4+1
Object:	? (SIMBAD class: PartofCloud = Part of Cloud)
in source:	X Cyg X-5
Ref:	=1983ApJ...273..219H
by	HESTER J.J. , PARKER R.A.R., DUFOUR R.J.
	Astrophys. J., 273, 219-242 (1983)
	Digital analysis of narrow-band imagery of the Cygnus Loop.
o	Fig.2, Table 4: <[HPD83] Star A> (Nos A-C). Fig.15: <[HPD83] Region R> (Nos I-IV), <[HPD83] Spur> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HPESL
HPESL	(Herschel/PACS Extended Source List) (Not yet in Simbad)
Write:	<<HPESL NNNA JHHMMSS.s+DDMMSS>> <<HPESL NNNA_JHHMMSS.s+DDMMSS>> (not recognised by Simbad, but found in literature)
N:	546587
Object:	(FIR) (SIMBAD class: FarIR = Far-IR source (λ >= 30 µm))
Note:	Herschel PACS observations of N=546587 slightly extended sources, extracted with the pipeline used for the Herschel/PACS Point Source Catalogue (HPPSC). In the format, NNN represents the wavelength in units of µm (070, 100, or 160 µm), and the letter A indicates the version of the catalogue ("A" being the first version). For more information, visit: https://www.cosmos.esa.int/web/herschel/pacs-point-source-catalogue See also HPPSC and HPRSL for the point source catalogue and the rejected source list respectively.
Ref:	=arXiv:1705.05693
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HPF2005]
[HPF2005]	(Hill+Prochaska+Fox+, 2006)
Write:	<<[HPF2005] GRB 051111 abs N.NN>>
N:	1
Object:	Absorber
Note:	Keck HIRES observations of GRB 051111.
Ref:	=2005GCN..4255....1H
by	HILL G. , PROCHASKA J.X., FOX D., SCHAEFER B., REED M.
	GRB Coordinates Network, Circular Service, 4255, 1-None (2005)
	GRB 051111: Keck HIRES redshift.
o	<[HPF2005] GRB 051111 abs N.NN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPF97]
[HPF97]	(Howard+Pipher+Forrest, 1997)= (IRS)
Write:	<<[HPF97] NN>> <<[HPF97] IRS N>> <<[HPF97] IRS Na>> <<[HPF97] IRS Nb>>
N:	81+9
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	In the format 'IRS Na' the letter 'a' stands for the brighter source in the double source 'N', the letter 'b' for the fainter one. See also [BBW79].
in source:	SH 2-255
Ref:	=1997ApJ...481..327H
by	HOWARD E.M. , PIPHER J.L., FORREST W.J.
	Astrophys. J., 481, 327-342 (1997)
	S255-2: The formation of a stellar cluster.
o	S255-2 = [SB86] S255 2
o	Table 2: <[HPF97] NN> (Nos 1-81), <[HPF97] IRS Na> (Nos 1-3, 1a-1b)
Ref:	=1999AcASn..40..364Y
by	YAO Y.-Q. , SATO S.
	Acta Astron. Sinica, 40, 364-375 (1999)
	Near infrared polarimetry of S255 IR complex.
o	Figs 2, 3: <[HPF97] IRS Na> (Nos 2a-2b, 3a-3b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPF98]
[HPF98]	(Howard+Pipher+Forrest, 1998)
Write:	<<[HPF98] NN>>
N:	63
Object:	* (SIMBAD class: Star)
in source:	[NS84] 14
Ref:	=1998ApJ...509..749H
by	HOWARD E.M. , PIPHER J.L., FORREST W.J.
	Astrophys. J., 509, 749-760 (1998)
	A near-infrared study of the NS 14 bipolar nebula.
o	Trapezium stars A to D = [NSM89] A to D
o	Table 2: <[HPF98] NN> (Nos 1-63).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPG94]
[HPG94]	(Heindl+Prince+Grunsfeld, 1994)
Write:	<<[HPG94] N>>
N:	5
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI and PSPC and VLA observations of the field around 1E 1740.7-2942.
Ref:	=1994ApJ...430..829H
by	HEINDL W.A. , PRINCE T.A., GRUNSFELD J.M.
	Astrophys. J., 430, 829-833 (1994)
	Observations of 1E 1740.7-2942 with ROSAT and the VLA.
o	Table 2: <[HPG94] N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPH2009]
[HPH2009]	(Hodges-Kluck+Pound+Harris+, 2009)= ([HPH2009a])
Write:	<<[HPH2009] NNa>>
N:	24
Object:	Clump (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	HCN and HCO+ (CARMA) and 12CO (JCMT) observations toward 1E 1740.7-2942.
in source:	1E 1740.0-2942
Ref:	=2009ApJ...696.1374H
by	HODGES-KLUCK E. , POUND M.W., HARRIS A.I., LAMB J.W., HODGES M.
	Astrophys. J., 696, 1374-1384 (2009)
	Dense, parsec-scale clumps near the Great Annihilator.
o	Table 2: <[HPH2009] NNa> N=24 among (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPH2009a]
[HPH2009a]	(Hodges-Kluck+Pound+Harris+, 2009)
*****	Avoid the usage of [HPH2009a], prefer [HPH2009]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPH2009b]
[HPH2009b]	(Henze+Pietsch+Haberl+, 2009)
Write:	<<[HPH2009b] SSN>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton, Chandra and Swift observations of the centre region of M31.
in source:	M 31:Bol 111 = Bol 111
in source:	M 31:Bol 194 = Bol 194
Ref:	=2009A&A...500..769H
by	HENZE M. , PIETSCH W., HABERL F., SALA G., QUIMBY R., HERNANZ M., DELLA VALLE M., MILNE P., WILLIAMS G.G., BURWITZ V., GREINER J., STIELE H., HARTMANN D.H., KONG A.K.H., HORNOCH K.
	Astron. Astrophys., 500, 769-779 (2009)
	The first two transient supersoft X-ray sources in M 31 globular clusters and the connection to classical novae.
o	Text: <[HPH2009b] SSN> (Nos SS1-SS2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPH2013]
[HPH2013]	(Hofmann+Pietsch+Henze+, 2013)
Write:	<<[HPH2013] NNN>>
N:	318
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra HRC-I observations of N=318 X-ray point sources in the central field of M 31.
in source:	M 31 = NGC 224
Ref:	=2013A&A...555A..65H
by	HOFMANN F. , PIETSCH W., HENZE M., HABERL F., STURM R., DELLA VALLE M., HARTMANN D.H., HATZIDIMITRIOU D.
	Astron. Astrophys., 555A, 65-65 (2013)
	X-ray source variability study of the M 31 central field using Chandra HRC-I.
o	Table 1: <[HPH2013] NNN> (Nos 1-318).
=E=	Catalogue in electronic form as J/A+A/555/A65
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPH2015]
[HPH2015]	(Hui+Park+Hu+, 2015)
Write:	<<[HPH2015] JHHMM XNN>> <<[HPH2015] JHHMM_XNN>> (not recognised by Simbad, but found in literature)
N:	20
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	N=20 X-ray sources in the field of six millisecond pulsar (MSPs) candidates, found in XMM-Newton, Chandra, and Swift archival data.
Ref:	=2015ApJ...809...68H
by	HUI C.Y. , PARK S.M., HU C.P., LIN L.C.C., LI K.L., KONG A.K.H., TAM P.H.T., TAKATA J., CHENG K.S., JIN R., YEN T.-C., KIM C.
	Astrophys. J., 809, 68 (2015)
	Searches for millisecond pulsar candidates among the unidentified Fermi objects.
o	Tables 3-5: possible optical counterparts of [HPH2015] JHHMM XNN are not in SIMBAD.
o	Figs 2-4+8-10, Table 2: <[HPH2015] JHHMM XNN> N=20.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPH2020]
[HPH2020]	(Herrera+Pety+Hughes+, 2020)
Write:	<<[HPH2020] LNN>>
N:	10
Object:	CO Cloud (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 6 and VLT MUSE observations of the N=10 most CO luminous clouds in the disk of NGC 628.
in source:	M 74 = NGC 628
Ref:	=2020A&A...634A.121H
by	HERRERA C.N. , PETY J., HUGHES A., MEIDT S.E., KRECKEL K., QUEREJETA M., SAITO T., LANG P., JIMENEZ-DONAIRE M.J., PESSA I., CORMIER D., USERO A., SLIWA K., FAESI C., BLANC G.A., BIGIEL F., CHEVANCE M., DALE D.A., GRASHA K., GLOVER S.C.O., HYGATE A.P.S., KRUIJSSEN J.M.D., LEROY A.K., ROSOLOWSKY E., SCHINNERER E., SCHRUBA A., SUN J., UTOMO D.
	Astron. Astrophys., 634A, 121-121 (2020)
	The headlight cloud in NGC 628: An extreme giant molecular cloud in a typical galaxy disk.
o	Fig. 1, Table 2: <[HPH2020] LNN> (Nos L1-L10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPJ88]
[HPJ88]	(Humphreys+Pennington+Jones+, 1988)
Write:	<<[HPJ88] R-NNNa>> <<[HPJ88] IIIR-NNNa>>
N:	203+107
Object:	Red * (SIMBAD class: Star)
Note:	Table I: In the format, the letter 'R' stands for candidate 'Red' * (Nos R-1 to R-200), 3 have 2 components a and b, N=203 Red candidates in M 31 (Nos IIIR-1 to IIIR-106), 1 has 2 components a and b, N=106 Red candidates in Baade field III Maps: plates 113-117
in source:	M 31 = NGC 224
Ref:	=1988AJ.....96.1884H
by	HUMPHREYS R.M. , PENNINGTON R.L., JONES T.J., GHIGO F.D.
	Astron. J., 96, 1884-1907 (1988)
	The red supergiants in M 31 : spectra, colors and luminosities.
o	Var. 4, 32 = [BS63] V3, V32
o	Table I: <[HPJ88] A-NNNa> N =203, (Nos R-1 to R-200), <[HPJ88] IIIA-NNNa> N=107, (Nos IIIR-1 to IIIR-106)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPM2006]
[HPM2006]	(Homeier+Postman+Menanteau+, 2006)
Write:	<<[HPM2006] Cl JHHMM+DDMM NNNNN>> <<[HPM2006] MS 1054.4-0321 NNNN>>
N:	9+12+23+12+21+13+32+35
Object:	G in ClG + G (SIMBAD class: Galaxy)
Note:	HST ACS observations of galaxies in 4 clusters.
in source:	ClG J1604+4304
in source:	ClG J1604+4321
in source:	ClG J0152-1357 = RX J0152.7-1357
in source:	1E 1054.4-0321 = ClG 1054-0321
Ref:	=2006AJ....131..143H
by	HOMEIER N.L. , POSTMAN M., MENANTEAU F., BLAKESLEE J.P., MEI S., DEMARCO R., FORD H.C., ILLINGWORTH G.D., ZIRM A.
	Astron. J., 131, 143-157 (2006)
	Imprints of environment on cluster and field late-type galaxies at z~1.
o	Tables 1, 2: <[HPM2006] Cl J1604+4304 NNNN> N=9+12. Tables 3, 4: <[HPM2006] Cl J1604+4321 NNNN> N=23+12. Tables 5, 6: <[HPM2006] MS 1054.4-0321 NNNN> N=32+35. Tables 7, 8: <[HPM2006] Cl J0152-1357 NNNNN> N=21+13.
=E=	Catalogue in electronic form as J/AJ/131/143
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPM94]
[HPM94]	(Hamuy+Phillips+Maza+, 1994)
Write:	<<[HPM94] SN 1992K N>>
N:	6
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	see also [HMP93] and [HPS96]
Ref:	=1994AJ....108.2226H
by	HAMUY M. , PHILLIPS M.M., MAZA J., SUNTZEFF N.B., DELLA VALLE M., DANZIGER J., ANTEZANA R., WISCHNJEWSKY M., AVILES R., SCHOMMER R.A., KIM Y.-C., WELLS L.A., RUIZ M.T., PROSSER C.F., KRZEMINSKI W., BAYLIN C.D., HARTIGAN P., HUGHES J.
	Astron. J., 108, 2226-2232 (1994)
	SN 1992K: a twin to the subluminous type Ia SN 1991bg.
o	Table 2: <[HPM94] SN 1992K N> (Nos 1-6)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPM99]
[HPM99]	(Haberl+Pietsch+Motch, 1999)
Write:	<<[HPM99] A>>
N:	9
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	ESO-NTT-SUSI2 and VLT FORS observations of the field of RX J0420.0-5022. N=9 objects in or close to the HRI error circle. One object (I) within the Chandra error circle.
Ref:	=1999A&A...351L..53H
by	HABERL F. , PIETSCH W., MOTCH C.
	Astron. Astrophys., 351, 53-57 (1999)
	RX J0420.0-5022: an isolated neutron star candidate with evidence for 22.7s X-ray pulsations.
o	Fig.3, Table 2: <[HPM99] A> (Nos A-H).
Ref:	=2004A&A...424..635H
by	HABERL F. , MOTCH C., ZAVLIN V.E., REINSCH K., GAENSICKE B.T., CROPPER M., SCHWOPE A.D., TUROLLA R., ZANE S.
	Astron. Astrophys., 424, 635-645 (2004)
	The isolated neutron star X-ray pulsars RX J0420.0-5022 and RX J0806.4-4123: New X-ray and optical observations.
o	Fig.7, Table 6: <[HPM99] A> (No. I) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HPPSC
HPPSC	(Herschel/PACS Point Source Catalogue) (Not yet in Simbad)
Write:	<<HPPSC NNNA JHHMMSS.s+DDMMSS>> <<HPPSC NNNA_JHHMMSS.s+DDMMSS>> (not recognised by Simbad, but found in literature)
N:	108319+131322+251392
Object:	(FIR) (SIMBAD class: FarIR = Far-IR source (λ >= 30 µm))
Note:	The Herschel/PACS Point Source Catalogue (HPPSC) is a FIR catalogue based on the broad-band photometric observations of the PACS instrument with filters centred at 70, 100 and 160 µm. In the format, NNN represents the wavelength in units of µm, and the letter A indicates the version of the catalogue ("A" being the first version). For more information, visit: https://www.cosmos.esa.int/web/herschel/pacs-point-source-catalogue See also HPESL and HPRSL for the extended and rejected source lists respectively.
Ref:	=arXiv:1705.05693
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HPRA
HPRA	(Haro+Parsamian, RAfaga (spanish))= (FSO) = (HFS1) = (T) = (Ton)
Write:	<<HPRA NNN>>
N:	359
Object:	Flare * (SIMBAD class: Eruptive* = Eruptive Variable)
Note:	Nos 255, 256, 258, 259, 299-325 are missing. For Nos 177-179 see also Haro+ 1969 Bol. Obs. Ton. Tac. 12, 33 For Nos 340-359 see also Chavira+ 1992IBVS.3764....1C Maps
in source:	NAME Orion Nebula
Ref:	=1968SSS.....7..141H
by	HARO G.
	Stars and stellar systems., 7, 141-None (1968)
	Flare stars.
o	Nebulae and interstellar matter, 1968, Ed. Middlehurst B.M., Serie Stars and stellar systems, vol. 7, p. 141.
o	Table 1: <HPRA NNN> (Nos 1-176). Table 4: <HFS4 NN> (Nos 1-11).
Ref:	=1969BOTT....5...59H
by	HARO G. , CHAVIRA E.
	Bol. Obs. Tonantz. Tacub., 5, 59-78 (1969)
	Flare stars in the Orion Nebula region.
o	<HPRA NNN> (Nos 177-254)
Ref:	=1978BITon...2..341P
by	PARSAMIAN E. , CHAVIRA E., GONZALEZ G.
	Bol. Inst. Tonantzintla, 2, 341-343 (1978)
	Flare stars in the Orion nebula region.
o	<HPRA NNN> (Nos 257, 260, 326-329)
Ref:	=1991RMxAA..22...15C
by	CHAVIRA E. , PARSAMIAN E.
	Rev. Mex. Astron. Astrofis., 22, 15-17 (1991)
	New flare stars and repetitions in the Orion association region.
o	R 6 = [TTT80] 6, AB NNN = KKO NNN
o	<HPRA NNN> (Nos 261-298)
Ref:	=1993RMxAA..25...71P
by	PARSAMIAN E.S. , CHAVIRA E., GONZALEZ G.
	Rev. Mex. Astron. Astrofis., 25, 71-73 (1993)
	New flare stars and repetitions in the Orion association region. II.
o	<HPRA NNN> (Nos 340-359).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HPRSL
HPRSL	(Herschel/PACS Rejected Source List) (Not yet in Simbad)
Write:	<<HPRSL NNNNNNN>>
N:	7185160
Object:	(FIR) (SIMBAD class: FarIR = Far-IR source (λ >= 30 µm))
Note:	Herschel PACS observations of N=7185160 sources, extracted with the pipeline used for the Herschel/PACS Point Source Catalogue (HPPSC) but rejected because they fail to pass one or more of the quality criteria. For more information, visit: https://www.cosmos.esa.int/web/herschel/pacs-point-source-catalogue See also HPPSC and HPESL for the point source catalogue and the extended source list respectively.
Ref:	=arXiv:1705.05693
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HPS
HPS	(HETDEX Pilot Survey)
Write:	<<HPS NNN>>
N:	479
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	McDonald 2.7m telescope VIRUS-P observations of N=479 emission-line galaxies, as a pilot survey for the Hobby-Eberly Telescope Dark Experiment.
Ref:	=2011ApJS..192....5A
by	ADAMS J.J. , BLANC G.A., HILL G.J., GEBHARDT K., DRORY N., HAO L., BENDER R., BYUN J., CIARDULLO R., CORNELL M.E., FINKELSTEIN S.L., FRY A., GAWISER E., GRONWALL C., HOPP U., JEONG D., KELZ A., KELZENBERG R., KOMATSU E., MacQUEEN P.J., MURPHY J., ODOMS P.S., ROTH M., SCHNEIDER D.P., TUFTS J.R., WILKINSON C.P.
	Astrophys. J., Suppl. Ser., 192, 5 (2011)
	The HETDEX pilot survey. I. Survey design, performance, and catalog of emission-line galaxies.
o	Tables 3-4: <HPS NNN> (Nos 1-479).
=E=	Catalogue in electronic form as J/ApJS/192/5
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HPS2012]
[HPS2012]	(Haines+Pereira+Sanderson+, 2012)
Write:	<<[HPS2012] JHHMMSS.sss+DDMMSS.ss>>
N:	48 (SIMBAD class: AGN = Active Galaxy Nucleus)
Stat:	is completely incorporated in Simbad
Note:	Chandra X-ray and MMT Hectospec observations of AGN in N=18 galaxy clusters.
Ref:	=2012ApJ...754...97H
by	HAINES C.P. , PEREIRA M.J., SANDERSON A.J.R., SMITH G.P., EGAMI E., BABUL A., EDGE A.C., FINOGUENOV A., MORAN S.M., OKABE N.
	Astrophys. J., 754, 97 (2012)
	LoCuSS: a dynamical analysis of X-ray active galactic nuclei in local clusters.
o	Table 2: <[HPS2012] JHHMMSS.sss+DDMMSS.ss> N=48
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPS93]
[HPS93]	(Hobson+Padman+Scott+, 1993)= (FIR)
Write:	<<[HPS93] FIR N>>
N:	4
Object:	(Far IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Table 4: (Nos 1-3). No. 4 added by Ward-Thompson, 1994, private communication, and found latter in the literature.
in source:	M 17:NAME M17SW = NAME M17SW
Ref:	=1993MNRAS.264.1025H
by	HOBSON M.P. , PADMAN R., SCOTT P.F., PRESTAGE R.M., WARD-THOMPSON D.
	Mon. Not. R. Astron. Soc., 264, 1025-1040 (1993)
	High-resolution millimetre and submillimetre continuum observations of M 17SW - II. Identification of embedded sources associated with H2O masers.
o	Table 4: <[HPS93] FIR N> (Nos 1-3)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPS96]
[HPS96]	(Hamuy+Phillips+Suntzeff+, 1996)
Write:	<<[HPS96] SN YYYYaa CNN>> <<[HPS96] SN YYYYA CNN>>
N:	239
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=239 stars around 32 SN. see also [HMP93] and [HPM94]
Ref:	=1996AJ....112.2408H
by	HAMUY M. , PHILLIPS M.M., SUNTZEFF N.B., SCHOMMER R.A., MAZA J., ANTEZANA R., WISCHNJEWSKY M., VALLADARES G., MUENA C., GONZALEZ L.E., AVILES R., WELLS L.A., SMITH R.C., NAVARRETE M., COVARRUBIAS R., WILLIGER G.M., WALKER A.R., LAYDEN A.C., ELIAS J.H., BALDWIN J.A., HERNANDEZ M., TIRADO H., UGARTE P., ELSTON R., SAAVEDRA N., BARRIENTOS F., COSTA E., LIRA P., RUIZ M.T., ANGUITA C., GOMEZ X., ORTIZ P., DELLA VALLE M., DANZIGER J., STORM J., KIM Y.-C., BAILYN C., RUBENSTEIN E.P., TUCKER D., CERSOSIMO S., MENDEZ R.A., SICILIANO L., SHERRY W., CHABOYER B., KOOPMANN R.A., GEISLER D., SARAJEDINI A., DEY A., TYSON N., RICH R.M., GAL R., LAMONTAGNE R., CALDWELL N., GUHATHAKURTA P., PHILLIPS A.C., SZKODY P., PROSSER C., HO L.C., McMAHAN R., BAGGLEY G., CHENG K.-P., HAVLEN R., WAKAMATSU K., JANES K., MALKAN M., BAGANOFF F., SEITZER P., SHARA M., STURCH C., HESSER J., HARTIGAN P., HUGHES J., WELCH D., WILLIAMS T.B., FERGUSON H., FRANCIS P.J., FRENCH L., BOLTE M., ROTH J., ODEWAHN S., HOWELL S., KRZEMINSKI W.
	Astron. J., 112, 2408-2437 (1996)
	BVRI light curves for 29 type Ia supernovae.
o	Table 3: <[HPS96] SN YYYYA CNN>, <[HPS96] SN YYYYaa CNN>, N=239
=E=	Catalogue in electronic form as J/AJ/112/2408
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPT2001]
[HPT2001]	(Hennebelle+Perault+Teyssier+, 2001)
Write:	<<[HPT2001] LL.ll+B.bb>>
N:	6
Object:	Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	ISO observations. See also Paper II: [THP2002].
Ref:	=2001A&A...365..598H
by	HENNEBELLE P. , PERAULT M., TEYSSIER D., GANESH S.
	Astron. Astrophys., 365, 598-611 (2001)
	Infrared dark clouds from the ISOGAL survey. Constraints on the interstellar extinction curve.
o	Table 1: <[HPT2001] LL.ll+B.bb> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HPW
HPW	(Hodge+Pyper+Webb)
Write:	<<HPW NN>> <<HPW R>>
N:	47+3
Object:	Dwarf G in ClG (SIMBAD class: Galaxy)
in source:	NAME Fornax Cluster
Ref:	=1965AJ.....70..559H
by	HODGE P.W. , PYPER D.M., WEBB C.J.
	Astron. J., 70, 559-563 (1965)
	Dwarf galaxies in the Fornax cluster.
o	Table I: <HPW NN> (Nos 1-47), <HPW R> (Nos I-III)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HPW2009]
[HPW2009]	(Hess+Pisano+Wilcots+, 2009) (Not yet in Simbad)
Write:	<<[HPW2009] Cloud N>> <<[HPW2009] HI Spur>> <<[HPW2009] HI Tail>>
N:	7
Object:	HI Cloud (SIMBAD class: HI = HI (21cm) Source)
Note:	HI observations of NGC 2997 with ATCA.
in source:	NGC 2997
Ref:	=2009ApJ...699...76H
by	HESS K.M. , PISANO D.J., WILCOTS E.M., CHENGALUR J.N.
	Astrophys. J., 699, 76-88 (2009)
	Anomalous H I in NGC 2997.
o	NGC 2297 is a misprint for NGC 2997.
o	Table 3: <[HPW2009] Cloud N> (Nos 1-5), <[HPW2009] HI Spur>, <[HPW2009] HI Tail>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HPY2007]
[HPY2007]	(Hakobyan+Petrosian+Yeghazaryan+, 2007)
Write:	<<[HPY2007] NN>>
N:	98
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Byurakan Observatory 2.6m telescope CIGAL Halpha/NII observations of NGC 6384.
in source:	NGC 6384
Ref:	=2007Ap.....50..426H
by	HAKOBYAN A.A. , PETROSIAN A.R., YEGHAZARYAN A.A., BOULESTEIX J.
	Ap, 50, 426-439 (2007)
	Study of the HII Regions in the Spiral Galaxy NGC6384.
o	Table 1: <[HPY2007] NN> (Nos 1-98).
=E=	Catalogue in electronic form as J/other/Ap/50.426
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HQ
HQ	(Havlen+Quintana)
Write:	<<HQ NN>>
N:	25
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Paper I, see also Paper II: QH
in source:	CA 0340-538 = ACO 3158
Ref:	=1978ApJ...220...14H
by	HAVLEN R.J. , QUINTANA H.
	Astrophys. J., 220, 14-18 (1978)
	Velocity dispersion and global parameters of the southern cluster of galaxies CA 0340-538 (= 3U 0328-52?).
o	Table 1: <HQ NN> (Nos 1-25)
Origin	of the Acronym: L (1981A&A....96..106C)
Details on Acronym: HQT
HQT	(Hawaii Quasar and T dwarf survey)
Write:	<<HQT NN>>
N:	10
Object:	QSO cand. + T dwarf cand. (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	The Hawaii Quasar and T dwarf survey (HQT survey) is a wide-field, red optical survey carried out with Subaru Suprime-Cam.
Ref:	=2010ApJ...723..184K
by	KAKAZU Y. , HU E.M., LIU M.C., WANG W.-H., WAINSCOAT R.J., CAPAK P.L.
	Astrophys. J., 723, 184-196 (2010)
	Hawaii quasar and T dwarf survey. I. Method and discovery of faint field ultracool dwarfs.
o	Tables 3-6: <HQT NN> (Nos 1-10).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HR
HR	(Hughes+Routledge) (Not yet in Simbad)
*****	Avoid the usage of HR, prefer [HR69]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HR
HR	(Harvard obs., Revised photometry)= BS = (BSC) = (RHP)
Write:	<<HR NNNN>> <<HR NNNNAA>> <<HR NNNNAa>>
N:	9110
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Discordances in star designations: 1979BICDS..17...38H.
Ref:	=1964BS....C......0H
by	HOFFLEIT D.
	The Bright Star Catalogue, 0-None (1964)
	Catalogue of bright stars. Third revised edition.
o	(Erratum) Bull. Inf. CDS 13, 14-23.
o	On magnetic tape.
o	<HR NNNN> N=9110.
Ref:	=1982BS....C......0H
by	HOFFLEIT D. , JASCHEK C., WARREN W.H.Jr, CHARLES E.H., HAUCK B.
	The Bright Star Catalogue, 0-None (1982)
	The bright stars catalogue. 4th revised edition.
o	(Erratum) WARREN W.H.Jr+, 1983, Bull. Inf. CDS 25, 49-50.
o	<HR NNNN> (Nos 1-9110).
Ref:	=1984BICDS..27..159W
by	WARREN W.H.
	Bull. Inf. Centre Donnees Stellaires, 27, 159-None (1984)
	Errata to the bright star catalogue.
o	<HR NNNN>
Ref:	=1984BICDS..27..161H
by	HOFFLEIT D.
	Bull. Inf. Centre Donnees Stellaires, 27, 161-195 (1984)
	Additions and corrections to the Bright Star catalogue.
o	<HR NNNN>
Ref:	=1992BICDS..40...71P
by	PETERS A.R. , HOFFLEIT D.E.
	Bull. Inf. Centre Donnees Stellaires, 40, 71-93 (1992)
	Some revisions to the Bright Star Catalogue and its supplement.
=E=	Catalogue in electronic form as V/50
=E=	Catalogue in electronic form as V/36
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HR
HR	(Hu+Ridgway)
*****	Avoid the usage of HR, prefer [HR94]
Origin	of the Acronym: L (1999ApJ...519..610D)
Details on Acronym: [HR2000]
[HR2000]	(Hagen+Reimers, 2000)
Write:	<<[HR2000] A>>
N:	2+4
Object:	QSO + G (SIMBAD class: Galaxy)
Note:	Fig.1: The double lensed QSO HS 0818+1227 has two components, (Nos A-B). The component B is contamined by the lensing galaxy 'G', which at the resolution used cannot be separated from B. The double QSO is located at the end of a chain of 3 galaxies, (Nos C-E). The component B is contamined by a galaxy 'G', which at the resolution used cannot be separated from B.
in source:	HS 0818+1227
Ref:	=2000A&A...357L..29H
by	HAGEN H.-J. , REIMERS D.
	Astron. Astrophys., 357, 29-31 (2000)
	HS 0818+1227: discovery of a new double gravitationally lensed QSO.
o	Fig.1, text: <[HR2000] A> (Nos A-E, G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HR2010]
[HR2010]	(Haikala+Reipurth, 2010)
Write:	<<[HR2010] NNN>> <<[HR2010] JHHMMSS.ss+DDMMSS.s>> <<[HR2010] W77-6a>>
N:	227
Object:	* (SIMBAD class: Star)
Note:	NTT SOFI NIR observations of CG 12.
in source:	NAME CG 12 Cluster
in source:	CG 12
Ref:	=2010A&A...510A...1H
by	HAIKALA L.K. , REIPURTH B.
	Astron. Astrophys., 510A, 1-1 (2010)
	Near infrared imaging of the cometary globule CG 12.
o	In ref list 1977 Williams MNRAS, 181, 179 is a misprint for 1977 Williams MNRAS, 180, 709.
o	Text: <NAME CG 12 cluster>. Table 1: <[HR2010] NNN> (Nos 1-227) = <[HR2010] JHHMMSS.ss+DDMMSS.s> N=227. Paragr. 4.1.4: <[HR2010] W77-6a> (Nos a-b).
=E=	Catalogue in electronic form as J/A+A/510/A1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HR69]
[HR69]	(Hughes+Routledge, 1969)= (HR) (Not yet in Simbad)
Write:	<<[HR69] NN>>
N:	55
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1969AJ.....74..604H
by	HUGHES V.A. , ROUTLEDGE D.
	Astron. J., 74, 604-607 (1969)
	A detailed survey of the galactic plane at a wavelength of 9.26 cm between longitudes 32° and 49°.
o	Objects [HR69] not in SIMBAD
o	<[HR69] NN> (Nos 1-55)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HR74]
[HR74]	(Hargrave+Ryle, 1974)
Write:	<<[HR74] A>> <<[HR74] Wa>>
N:	6+3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	HST archive data. Radio hotspots in Cyg A.
in source:	Cyg A = 3C 405
Ref:	=1974MNRAS.166..305H
by	HARGRAVE P.J. , RYLE M.
	Mon. Not. R. Astron. Soc., 166, 305-327 (1974)
	Observations of Cygnus A with the 5km radio telescope.
o	Table I: <[HR74] A> (Nos A-D), <[HR74] Wa> (Nos Np, Sf, Ce)
Ref:	=1984MNRAS.209..851A
by	ALEXANDER P. , BROWN M.T., SCOTT P.F.
	Mon. Not. R. Astron. Soc., 209, 851-868 (1984)
	A multi-frequency radio study of Cygnus A.
o	Figs 1, 2: <[HR74] A> (Nos E, F) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HR89]
[HR89]	(Huchtmeier+Richter, 1989) (Not yet in Simbad)
Write:	<<[HR89] Anon HHMM+DDa>>
Object:	G (SIMBAD class: Galaxy)
Note:	From the 'General catalog of HI observations of galaxies. The reference catalogue.' by Huchtmeier + Richter, 1989. The acronym is created for galaxies designated as 'Anon HHMM+DDa' coming from the RC2 catalogue of De Vaucouleurs.
Auth.:	HUCHTMEIER W.K.+
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HR92]
[HR92]	(Heathcote+Reipurth, 1992)
Write:	<<[HR92] NN>>
N:	44
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1992AJ....104.2193H
by	HEATHCOTE S. , REIPURTH B.
	Astron. J., 104, 2193-2212 (1992)
	Kinematics and evolution of the HH 34 complex.
o	Table 2: <[HR92] NN> (Nos 1-44)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HR94]
[HR94]	(Hu+Ridgway, 1994)= (HR)
Write:	<<[HR94] NN>>
N:	19
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	[HR94] 10 and [HR94] 14 are the two extremely red galaxies. [HR94] 7 is a QSO.
Ref:	=1994AJ....107.1303H
by	HU E.M. , RIDGWAY S.E.
	Astron. J., 107, 1303-1306 (1994)
	Two extremely red galaxies.
o	<[HR94] NN> N=19
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HRB2007]
[HRB2007]	(Harvey+Rebull+Brooke+, 2007)
Write:	<<[HRB2007] JHHMMSS.s+DDMMSS>> <<[HRB2007] A>>
N:	4+3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Spitzer MIPS observations of the Serpens Cloud. See also [HMH2007].
in source:	NAME Serpens Cloud
Ref:	=2007ApJ...663.1139H
by	HARVEY P.M. , REBULL L.M., BROOKE T., SPIESMAN W.J., CHAPMAN N., HUARD T.L., EVANS II N.J., CIEZA L., LAI S.-P., ALLEN L.E., MUNDY L.G., PADGETT D.L., SARGENT A.I., STAPELFELDT K.R., MYERS P.C., VAN DISHOECK E.F., BLAKE G.A., KOERNER D.W.
	Astrophys. J., 663, 1139-1148 (2007)
	The Spitzer c2d survey of large, nearby, interstellar clouds. VIII. Serpens observed with MIPS.
o	Table 3: <[HRB2007] JHHMMSS.s+DDMMSS> N=4. Table 7: <[HRB2007] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HRB2013]
[HRB2013]	(Herrera+Rubio+Bolatto+, 2013)
Write:	<<[HRB2013] NN>>
N:	19
Object:	CO Cloud (SIMBAD class: MolCld = Molecular Cloud)
Note:	SEST SIMBA CO(2-1) line observations of N=19 molecular clouds in the N11 star-forming region in the LMC.
Ref:	=2013A&A...554A..91H
by	HERRERA C.N. , RUBIO M., BOLATTO A.D., BOULANGER F., ISRAEL F.P., RANTAKYROE F.T.
	Astron. Astrophys., 554A, 91-91 (2013)
	Millimeter dust emission compared with other mass estimates in N11 molecular clouds in the LMC.
o	Table 2: <[HRB2013] NN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HRB81]
[HRB81]	(Haschick+Reid+Burke+, 1981)
Write:	<<[HRB81] W75N(A)>> <<[HRB81] W75N(Aa)>> <<[HRB81] W75N(H2O)>> <<[HRB81] W75N(OH)>> <<[HRB81] W75N(CO)>> <<[HRB81] W75N(HCN)>> <<[HRB81] W75N(IR)>>
N:	3+4+5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio continuum sources in W 75N: N=3 sources (Nos A-C), named [HRB1] W75N(A) to C, [HRB1] W75N(B) been divided into 4 components [HRB1] W75N(Ba) to [HRB1] W75N(Bd). N=5 sources in H2O, OH, CO, HCN, and IR
in source:	W 75:W 75N = W 75N
Ref:	=1981ApJ...244...76H
by	HASCHICK A.D. , REID M.J., BURKE B.F., MORAN J.M., MILLER G.
	Astrophys. J., 244, 76-87 (1981)
	VLBI aperture synthesis observations of the OH maser source W75N.
o	Table 2: <[HRB81] W75N(A)> (Nos A-C), <[HRB81] W75N(H2O)>, <[HRB81] W75N(OH)>, <[HRB81] W75N(CO)>, <[HRB81] W75N(HCN)>, <[HRB81] W75N(IR)>
Ref:	=1994A&A...284..215H
by	HUNTER T.R. , TAYLOR G.B., FELLI M., TOFANI G.
	Astron. Astrophys., 284, 215-226 (1994)
	Water masers embedded in ultracompact HII regions : the W 75N cloud core.
o	Table 1: <[HTF94] W75N N> (Nos 1-5). Table 2, Fig.1: <[HRB81] W75N(Ba)> (Nos Ba-Bd).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HRB97]
[HRB97]	(Herbst+Robberto+Beckwith, 1997) (Not yet in Simbad)
Write:	<<[HRB97] A>>
N:	16
Object:	Filament (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Fig.8: N=16 molecular hydrogen structures near T Tau
in source:	V* T Tau
Ref:	=1997AJ....114..744H
by	HERBST T.M. , ROBBERTO M., BECKWITH S.V.W.
	Astron. J., 114, 744-756 (1997)
	Wind disk-ambient cloud interactions in the near environment of T Tauri.
o	Fig.:8: <[HRB97] A> (Nos A-R, N and O missing)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HRC
HRC	(Herbig+Rao, Catalog)
Note:	subset of HBC (ref. 1988LicOB1111......1H), use acronym HBC
*****	Avoid the usage of HRC, prefer HBC
Details on Acronym: HRC
HRC	(Hamburg-RASS Catalogue)
*****	Avoid the usage of HRC, prefer [ZEH2003]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HRDS
HRDS	(HII Region Discovery Survey)
Write:	<<HRDS GLLL.lll+BB.bbb>>
N:	448+37
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	The HII Region Discovery Survey (HRDS) is a survey of recombination line and continuum emission at X-band (9GHz, 3cm), made with the Green Bank Telescope (GBT) and the Arecibo Observatory. It extends from 343°<l<67°, \|b\|<1°. N=485 HII regions (448 with the GBT and 37 with Arecibo) have been detected. See also the survey website http://www.cv.nrao.edu/hrds
Ref:	=2011ApJS..194...32A
by	ANDERSON L.D. , BANIA T.M., BALSER D.S., ROOD R.T.
	Astrophys. J., Suppl. Ser., 194, 32 (2011)
	The Green Bank Telescope H II Region Discovery Survey. II. The source catalog.
o	Table 1: <HRDS GLLL.lll+B.bbb> N=448.
Ref:	=2012ApJ...759...96B
by	BANIA T.M. , ANDERSON L.D., BALSER D.S.
	Astrophys. J., 759, 96 (2012)
	The Arecibo H II Region Discovery Survey.
o	Fig. 1, Table 1: <HRDS GLLL.lll+BB.bbb> N=37. Paragr. 6.3 and 6.4: <[BAB2012] GNN> (Nos G46, G52), <[BAB2012] G52L> N=1.
=E=	Catalogue in electronic form as <J/ApJS/194/32/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HRF2005]
[HRF2005]	(Hatchell+Richer Fuller+, 2005)
Write:	<<[HRF2005] NN>>
N:	91
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SCUBA at JCMT maps of the submm dust emission from the Perseus molecular cloud: 91 embedded starless and protostellar cores and filamentary structures are found. See also [HFR2007].
in source:	NAME Perseus Molecular Cloud
Ref:	=2005A&A...440..151H
by	HATCHELL J. , RICHER J.S., FULLER G.A., QUALTROUGH C.J., LADD E.F., CHANDLER C.J.
	Astron. Astrophys., 440, 151-161 (2005)
	Star formation in Perseus. Clusters, filaments and the conditions for star formation.
o	Paragraph 5.1 IRAS 03422+3256 is a probable misprint for IRAS 03422+3156.
o	Table A1: <[HRF2005] NN> (Nos 1-91).
=E=	Catalogue in electronic form as J/A+A/440/151
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HRG
HRG	(Hertling, Ring Galaxy)
Write:	<<HRG FFFNN>>
N:	108+125
Object:	Ring G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Format 'FFFNN': always 5 digits without space or separator. The first three 'FFF' are ESO plate number, the two last 'NN' are ring galaxy running number in that plate.
Ref:	=1992A&AS...94..245F
by	FAUNDEZ-ABANS M. , HERTLING G., RAMIREZ A.C.
	Astron. Astrophys., Suppl. Ser., 94, 245-250 (1992)
	The visual appearance of the nuclei of ring-shaped galaxies as an alternative classification criterion.
o	ESO 159-02 misprint for 195-02
o	<HRG FFFNN> N=108, format with always 5 digits
Ref:	=1994A&AS..104....1F
by	FAUNDEZ-ABANS M. , CUEVAS H.L., HERTLING G.P.
	Astron. Astrophys., Suppl. Ser., 104, 1-7 (1994)
	Search for faint ring-shaped galaxies in the -77° to -87° declination interval.
o	positions could be wrong up to 10'. Positions are offen different in 1998A&AS..129..357F
o	<HRG FFFNN> N=125, format with always 5 digits
=E=	Catalogue in electronic form as J/A+AS/104/1
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HRG14
HRG14	(High Redshift Galaxy, 2014)
Write:	<<HRG14 JHHMMSS.ss+DDMMSS.s>>
N:	7446
Object:	G (SIMBAD class: Galaxy)
Note:	N=7446 candidate galaxies at 3.5<z<8.5 in the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey/GOODS fields, the Hubble Ultra Deep Field, and the Hubble Frontier Field (HFF) deep parallel observations near the Abell 2744 and MACS J0416.1-2403 clusters. Use of HST data from CANDELS, HUDF and HUDF09 surveys, and Frontier Fields program. See also <[FRP2015]>.
in source:	NAME GOODS South Field
in source:	NAME GOODS North Field
in source:	NAME HUDF
in source:	MCS J0416.1-2403
in source:	ACO 2744
Ref:	=2015ApJ...810...71F
by	FINKELSTEIN S.L. , RYAN R.E.Jr, PAPOVICH C., DICKINSON M., SONG M., SOMERVILLE R.S., FERGUSON H.C., SALMON B., GIAVALISCO M., KOEKEMOER A.M., ASHBY M.L.N., BEHROOZI P., CASTELLANO M., DUNLOP J.S., FABER S.M., FAZIO G.G., FONTANA A., GROGIN N.A., HATHI N., JAACKS J., KOCEVSKI D.D., LIVERMORE R., McLURE R.J., MERLIN E., MOBASHER B., NEWMAN J.A., RAFELSKI M., TILVI V., WILLNER S.P.
	Astrophys. J., 810, 71 (2015)
	The evolution of the galaxy rest-frame ultraviolet luminosity function over the first two billion years.
o	Table 3, col(2): <HRG14 JHHMMSS.ss+DDMMSS.s> N=7446 = Table 3, col(1): <[FRP2015] zN AAAAAAAAAAA NNNNN>, <[FRP2015] zN PARN NNNN>, N=7446.
=E=	Catalogue in electronic form as J/ApJ/810/71
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HRG2013]
[HRG2013]	(Hu+Richer+Gwyn+, 2013)
Write:	<<[HRG2013] JHHMMSS.ss+DDMMSS.s>>
N:	44
Object:	Poss. WD (SIMBAD class: WhiteDwarf_Candidate = White Dwarf Candidate)
Note:	Discovery of N=44 high proper motion white dwarfs in the deep survey of the Canada France Hawaii Telescope Legacy Survey (CFHTLS).
Ref:	=2013ApJ...766...46H
by	HU J.-H. , RICHER H., GWYN S.D.J., IP W.-H.
	Astrophys. J., 766, 46 (2013)
	Search for high proper motion objects in the CFHTLS deep fields.
o	Tables 1,3: <[HRG2013] JHHMMSS.ss+DDMMSS.s> N=44.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HRH2018]
[HRH2018]	(Huang+Riess+Hoffmann+, 2018)
Write:	<<[HRH2018] NNNNNN>>
N:	44+388
Object:	* + Poss. Mira (SIMBAD class: Star)
Note:	HST WFC3 observations of N=44 secondary stars and N=388 Mira candidates in NGC 4258.
in source:	NGC 4258
Ref:	=2018ApJ...857...67H
by	HUANG C.D. , RIESS A.G., HOFFMANN S.L., KLEIN C., BLOOM J., YUAN W., MACRI L.M., JONES D.O., WHITELOCK P.A., CASERTANO S., ANDERSON R.I.
	Astrophys. J., 857, 67-67 (2018)
	A near-infrared period-luminosity relation for Miras in NGC 4258, an anchor for a new distance ladder.
o	Tables 2+6: <[HRH2018] NNNNNN> N=44+388 among (Nos 695-271584).
=E=	Catalogue in electronic form as <J/ApJ/857/67/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HRH87]
[HRH87]	(Hartigan+Raymond+Hartmann, 1987)
Write:	<<[HRH87] Cep A-A>> <<[HRH87] Cep A-AW>> <<[HRH87] Cep A-W>>
N:	8+11+1
Object:	HH (SIMBAD class: HerbigHaroObj = Herbig-Haro Object)
Note:	HH objects in Cep A
in source:	NAME Cep A
Ref:	=1987ApJ...316..323H
by	HARTIGAN P. , RAYMOND J., HARTMANN L.
	Astrophys. J., 316, 323-348 (1987)
	Radiative bow shock models of Herbig-Haro objects.
o	Table 4: <[HRH87] Cep A-A> (Nos A-A to A-H), <[HRH87] Cep A-HW> N=1, <[HRH87] Cep A-S> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HRK
HRK	(Heiles+Reach+Koo, 1988)
Write:	<<HRK LLL.l+BB.b>>
N:	30
Object:	Cloud (SIMBAD class: Cloud)
Ref:	=1988ApJ...332..313H
by	HEILES C. , REACH W.T., KOO B.-C.
	Astrophys. J., 332, 313-327 (1988)
	Molecules, grains, and shocks : a comparison of CO, H I, and IRAS data.
o	Table 1: <HRK LLL.l+BB.b> N=30.
Origin	of the Acronym: L (1998ApJ...507..507R)
Details on Acronym: [HRL2018]
[HRL2018]	(Howk+Rueff+Lehner+, 2018)
Write:	<<[HRL2018] NGC 4013 EHR 1>> <<[HRL2018] NGC 4013 disk N>>
N:	1+2
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	LBT MODS1 observations of N=1 extraplanar HII region (EHR) and N=2 disk regions in NGC 4013.
in source:	NGC 4013
Ref:	=2018ApJ...856..166H
by	HOWK J.C. , RUEFF K.M., LEHNER N., WOTTA C.B., CROXALL K., SAVAGE B.D.
	Astrophys. J., 856, 166-166 (2018)
	Extraplanar H II regions in spiral galaxies. I. Low-metallicity gas accreting through the disk-halo interface of NGC 4013.
o	Fig. 1, Table 1: <[HRL2018] NGC 4013 EHR 1> N=1, <[HRL2018] NGC 4013 disk N> (Nos disk 1- disk 2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HRO
HRO	(Highly Red Object)
*****	Avoid the usage of HRO, prefer [KTV98]
Details on Acronym: [HRP2007]
[HRP2007]	(Huang+Rigopoulou+Papovich+, 2007)
Write:	<<[HRP2007] EGS20 J1418+5236>> <<[HRP2007] EGS20 J1418+5236 JN>>
N:	1+3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRS specroscopy of the LBG 'EGS20 J1418+5236'. N=2 HST ACS components J1 and J2 and another object J3 3" east.
Ref:	=2007ApJ...660L..69H
by	HUANG J.-S. , RIGOPOULOU D., PAPOVICH C., ASHBY M.L.N., WILLNER S.P., IVISON R., LAIRD E.S., WEBB T., WILSON G., BARMBY P., CHAPMAN S., CONSELICE C., McLEOD B., SHU C.G., SMITH H.A., LE FLOC'H E., EGAMI E., WILLMER C.N.A., FAZIO G.G.
	Astrophys. J., 660L, 69-72 (2007)
	AEGIS: infrared spectroscopy of an infrared-luminous Lyman break galaxy at z=3.01.
o	Fig.2: <[HRP2007] EGS20 J1418+5236> N=1, <[HRP2007] EGS20 J1418+5236 JN> (Nos J1-J3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HRR2000]
[HRR2000]	(Heydari-Malayeri+Royer+Rauw+, 2000)
Write:	<<[HRR2000] Sk -66 41 NN>> <<[HRR2000] HNT NNN>>
N:	18+70
Object:	* in Cl* (SIMBAD class: Star)
Note:	N=15 stars are members of Sk -66 41 Cluster among (Nos 1-57) in the field of the cluster. N=70 stars are members of HNT Cluster, (Nos 61-130). See also [HMR88], [HB94], HNT.
in source:	NAME SK -66 41 Cluster
in source:	HNT Cluster
Ref:	=2000A&A...361..877H
by	HEYDARI-MALAYERI M. , ROYER P., RAUW G., WALBORN N.R.
	Astron. Astrophys., 361, 877-887 (2000)
	Compact star clusters of the LMC HII region N11C.
o	(Erratum) Erratum 2000 A&A Vol 364, p. 923.
o	Table 1, text: <[HRR2000] Sk -66 41 NN> N=18 among (Nos 1-57). Table 2, text: <[HRR2000] HNT NNN> (Nos 61-130).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HRR2004]
[HRR2004]	(Hessels+Roberts+Ramson+, 2004)
Write:	<<[HRR2004] JHHMMSS.ss+DDMMSS.s>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-S observation of PSR J2021+3651 and its X-ray PWN (Pulsar Wind Nebula) NAME PWN 75.2+0.1. 2 X-ray point sources are observed, the first embedded in the nebula, the second corresponding to an optical USNO-B1.0 star.
Ref:	=2004ApJ...612..389H
by	HESSELS J.W.T. , ROBERTS M.S.E., RANSOM S.M., KASPI V.M., ROMANI R.W., NG C.-Y., FREIRE P.C., GAENSLER B.M.
	Astrophys. J., 612, 389-397 (2004)
	Observations of PSR J2021+3651 and its X-ray pulsar wind nebula G75.2+0.1.
o	Text: <[HRR2004] JHHMMSS.ss+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HRR77]
[HRR77]	(Herbst+Racine+Richer, 1977)
Write:	<<[HRR77] NN>>
N:	27
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	NAME ASS CMA OB 1-
Ref:	=1977PASP...89..663H
by	HERBST W. , RACINE R., RICHER H.B.
	Publ. Astron. Soc. Pac., 89, 663-667 (1977)
	A luminous carbon star in Canis Major OB1.
o	Table I: <[HRR77] NN> (Nos 1-27).
Origin	of the Acronym: L (1997BaltA...6..499B)
Details on Acronym: HRS
HRS	(Herschel Reference Sample)
*****	Avoid the usage of HRS, prefer [BEC2010]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HRS
HRS	(Horologium-Reticulum Supercluster)
Write:	<<HRS JHHMMSS+DDMMSS>>
N:	546+2
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Observations of the Horologium-Reticulum Supercluster with the 6deg field multifiber spectrograph on the UKST at the AAO.
in source:	NAME HOROLOGIUM-RETICULUM SUPERCL
Ref:	=2005AJ....130..957F
by	FLEENOR M.C. , ROSE J.A., CHRISTIANSEN W.A., HUNSTEAD R.W., JOHNSTON-HOLLITT M., DRINKWATER M.J., SAUNDERS W.
	Astron. J., 130, 957-967 (2005)
	Large-scale velocity structures in the Horologium-Reticulum supercluster.
o	Table 2: <HRS JHHMMSS+DDMMSS> N=546.
Ref:	=2006AJ....131.1280F
by	FLEENOR M.C. , ROSE J.A., CHRISTIANSEN W.A., JOHNSTON-HOLLITT M., HUNSTEAD R.W., DRINKWATER M.J., SAUNDERS W.
	Astron. J., 131, 1280-1287 (2006)
	Redshifts and velocity dispersions of galaxy clusters in the Horologium-Reticulum supercluster.
o	03 00 33.75 -51 47 43.9
o	Table 1: <HRS JHHMMSS+DDMMSS> N=2 added.
=E=	Catalogue in electronic form as J/AJ/130/957
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HRS2007]
[HRS2007]	(Hessels+Ransom+Stairs+, 2007)
Write:	<<[HRS2007] M 53 Psr A>> <<[HRS2007] M 3 Psr A>> <<[HRS2007] M 71 Psr A>> <<[HRS2007] NGC 6749 Psr A>>
N:	1+4+1+2
Object:	ms Psr (SIMBAD class: Pulsar)
Stat:	is completely incorporated in Simbad
Note:	Arecibo 1.4GHz observations of millisecond pulsars in 4 globular clusters.
in source:	M 53 = NGC 5024
in source:	M 3 = NGC 5272
in source:	M 71 = NGC 6838
in source:	NGC 6749
Ref:	=2007ApJ...670..363H
by	HESSELS J.W.T. , RANSOM S.M., STAIRS I.H., KASPI V.M., FREIRE P.C.C.
	Astrophys. J., 670, 363-378 (2007)
	A 1.4 GHz Arecibo survey for pulsars in globular clusters.
o	Tables 3, 4: <[AKP89] M 13 Psr A> (Nos B-E) added, <[WAK89] M 5 Psr A> (Nos C-E) added, <[HRS2007] M 53 Psr A> (No. A), <[HRS2007] M 3 Psr A> (Nos A-D), <[HRS2007] M 71 Psr A> (No. A), <[HRS2007] NGC 6749 Psr A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HRS2015]
[HRS2015]	(Hartigan+Reiter+Smith+, 2015)
Write:	<<[HRS2015] RN>> <<[HRS2015] PN?>> <<[HRS2015] Finger IRS>> <<[HRS2015] HHc-21>> <<[HRS2015] HHc-21 Star>>
N:	5+1+1+1+1
Object:	Cometary Globule + Poss. HH + Poss. PN + * (SIMBAD class: EmObj = Emission Object)
Note:	CTIO Blanco 4-m telescope NEWFIRM narrowband observations of the Carina Nebula.
in source:	NGC 3372 = Carina Nebula
Ref:	=2015AJ....149..101H
by	HARTIGAN P. , REITER M., SMITH N., BALLY J.
	Astron. J., 149, 101 (2015)
	A survey of irradiated pillars, globules, and jets in the Carina nebula.
o	Text: <MHO NNNN> (Nos 1606-1629) added, <HH NNNN> (Nos 1123-1128) added. Fig. 32, Table 2: <[HRS2015] RN> (Nos R1-R5), <[HRS2015] HHc-21> N=1, <[HRS2015] HHc-21 Star> N=1. Fig. 11, Table 2: <[HRS2015] PN?> N=1. Fig. 35, Table2: <[HRS2015] Finger IRS> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HRS96]
[HRS96]	(Hunsch+Reimers+Schmitt, 1996)
Write:	<<[HRS96] JHHMMSS.s+DDMMSS>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Ref:	=1996A&A...313..755H
by	HUENSCH M. , REIMERS D., SCHMITT J.H.M.M.
	Astron. Astrophys., 313, 755-758 (1996)
	HR 4289 - an X-ray luminous galaxy close to the bright star.
o	<[HRS96] J110011.0-140431> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HRT98]
[HRT98]	(Honeycutt+Robertson+Turner+, 1998)= ([HRT98a])
Write:	<<[HRT98] A>>
N:	3
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Stars [HRT98] B, C are found very close to V* V446 Her = [HRT98] A.
Ref:	=1998ApJ...495..933H
by	HONEYCUTT R.K. , ROBERTSON J.W., TURNER G.W., HENDEN A.A.
	Astrophys. J., 495, 933-940 (1998)
	V446 Herculis (Nova Her 1960) is an optical triple: implications for the resumption of dwarf nova outbursts following the nova.
o	[HRT98] A = V* V446 Her
o	Table 1: <[HRT98] A> (Nos A-C)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HRT98a]
[HRT98a]	(Honeycutt+Robertson+Turner+, 1998)
*****	Avoid the usage of [HRT98a], prefer [HRT98]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HRT98b]
[HRT98b]	(Haffner+Reynolds+Tufte, 1998) (Not yet in Simbad)
Write:	<<[HRT98b] Filament N>>
N:	2
Object:	Filament (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Discovery of 2 large faint filaments in our Galaxy.
Ref:	=1998ApJ...501L..83H
by	HAFFNER L.M. , REYNOLDS R.J., TUFTE S.L.
	Astrophys. J., 501, 83-88 (1998)
	Faint, large-scale Hα filaments in the Milky Way.
o	Table 1: <[HRT98b] Filament N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HRW
HRW	(Herbst+Racine+Warner)= (CMa R1)
Write:	<<HRW NNa>>
N:	37
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	HRW 1 = VDB 86 + VDB 87a + VDB 87b + VDB 87c. (Nos 1-31), +6 obj. NNa
in source:	NAME ASS CMA R 1-
Ref:	=1978ApJ...223..471H
by	HERBST W. , RACINE R., WARNER J.W.
	Astrophys. J., 223, 471-482 (1978)
	Optical and infrared properties of the newly formed stars in Canis Major R1.
o	Tables 1, 2: <HRW NNa> N=37
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HRY2009]
[HRY2009]	(Hinz+Rieke+Yusef-Zadeh+, 2009)
Write:	<<[HRY2009] DDD.dddddd+DD.ddddddd>>
N:	about 120000
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Spitzer MIPS 24mu.m observations.
in source:	NAME Gal Center
Ref:	=2009ApJS..181..227H
by	HINZ J.L. , RIEKE G.H., YUSEF-ZADEH F., HEWITT J., BALOG Z., BLOCK M.
	Astrophys. J., Suppl. Ser., 181, 227-232 (2009)
	A catalog of 24 µm sources toward the Galactic center.
o	Table 2: <[HRY2009] DDD.dddddd+DD.dddddd> N=about 120000.
=E=	Catalogue in electronic form as J/ApJS/181/227
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HRY2020]
[HRY2020]	(Huang+Riess+Yuan+, 2020)
Write:	<<[HRY2020] NNNNNN>>
N:	116
Object:	Mira (SIMBAD class: Mira = Mira Variable)
Note:	HST WFC3 observations of N=116 O-rich Mira variables in NGC 1559.
in source:	NGC 1559
Ref:	=2020ApJ...889....5H
by	HUANG C.D. , RIESS A.G., YUAN W., MACRI L.M., ZAKAMSKA N.L., CASERTANO S., WHITELOCK P.A., HOFFMANN S.L., FILIPPENKO A.V., SCOLNIC D.
	Astrophys. J., 889, 5-5 (2020)
	Hubble Space Telescope observations of Mira variables in the SN Ia host NGC 1559: an alternative candle to measure the Hubble constant.
o	Table 3: <[HRY2020] NNNNNN> N=116 among (Nos 158-332971).
=E=	Catalogue in electronic form as <J/ApJ/889/5/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HRZ99]
[HRZ99]	(Heydari-Malayeri+Rosa+Zinnecker+, 1999)
Write:	<<[HRZ99] NN>>
N:	19
Object:	* (SIMBAD class: Star)
Note:	HST WFPC2 observations. Table 1: Only brightest stars towards N81 (LHA 115-N 81) are in the table. See also [HMC2003]. Map in Fig.2
in source:	Magellanic Clouds:SMC:LHA 115-N 81 = LHA 115-N 81
Ref:	=1999A&A...344..848H
by	HEYDARI-MALAYERI M. , ROSA M.R., ZINNECKER H., DEHARVENG L., CHARMANDARIS V.
	Astron. Astrophys., 344, 848-856 (1999)
	Very young massive stars in the Small Magellanic Cloud, revealed by HST.
o	Table 1: <[HRZ99] NN> N=19 among 37.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HS
HS	(Henden+Stone) (Not yet in Simbad)
*****	Avoid the usage of HS, prefer FASTT
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HS
HS	(Hintzen+Scott) (Not yet in Simbad)
*****	Avoid the usage of HS, prefer [HS79]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HS
HS	(Haze (misprint for Gaze)+Shajn)
Note:	Ref. 1955IzKry..15...11G, erroneous translit. Haze for Gaze
*****	Avoid the usage of HS, prefer [GS55]
Details on Acronym: HS
HS	(Hamburg Schmidt survey)
Write:	<<HS HHMM+DDMMA>>
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Only specific first references are given: 1988A&A...195...15H: First ref. from the Hamburg Schmidt survey, N=1. 1995A&AS..111..195H: description of the HS survey. 1998A&AS..128..507E: 1st list of N=121 QSO. 1999A&AS..135..511U: 1st list of N=70 G.
Ref:	=1988A&A...195...15H
by	HAGEN H.-J. , GROOTE D., ENGELS D., TOUSSAINT F., REIMERS D.
	Astron. Astrophys., 195, 15-20 (1988)
	A new supergiant HII region in galaxy HS 1227+4758.
o	First ref. from this survey. In this ref. <HS HHMM+DDMMA> N=1
Ref:	=1998A&AS..128..507E
by	ENGELS D. , HAGEN H.-J., CORDIS L., KOEHLER S., WISOTZKI L., REIMERS D.
	Astron. Astrophys., Suppl. Ser., 128, 507-523 (1998)
	The Hamburg Quasar Survey. II. A first list of 121 quasars.
o	(Erratum) Erratum vol. 131, p. 196
o	Tables 2, 3, 4: <HS HHMM+DDMM> N=121
Ref:	=1999A&AS..135..511U
by	UGRYUMOV A.V. , ENGELS D., LIPOVETSKY V.A., HAGEN H.-J., HOPP U., PUSTIL'NIK S.A., KNIAZEV A.Y., RICHTER G., IZOTOV Y.I., POPESCU C.C.
	Astron. Astrophys., Suppl. Ser., 135, 511-529 (1999)
	The Hamburg/SAO Survey for Emission-Line Galaxies. I. A First List of 70 Galaxies.
o	Tables 1-5: <HS HHMM+DDMMA> N=70+4+7+111.
Ref:	=1999A&AS..137..299P
by	PUSTILNIK S.A. , ENGELS D., UGRYUMOV A.V., LIPOVETSKY V.A., HAGEN H.-J., KNIAZEV A.Y., IZOTOV Y.I., RICHTER G.
	Astron. Astrophys., Suppl. Ser., 137, 299-304 (1999)
	The Hamburg/SAO survey for emission-line galaxies. II. The second list of 128 galaxies.
o	Tables 2-6: <HS HHMM+DDMMA> N=128.
Ref:	=2000A&AS..142..417H
by	HOPP U. , ENGELS D., GREEN R.F., UGRYUMOV A.V., IZOTOV Y.I., HAGEN H.-J., KNIAZEV A.Y., LIPOVETSKY V.A., PUSTILNIK S.A., BROSCH N., MASEGOSA J., MARTIN J.-M., MARQUEZ I.
	Astron. Astrophys., Suppl. Ser., 142, 417-423 (2000)
	The Hamburg/SAO survey for emission-line galaxies. III. The third list of 81 galaxies.
o	Tables 2-6: <HS HHMM+DDMMA> N=81.
Ref:	=2001A&A...366..771K
by	KNIAZEV A.Y. , ENGELS D., PUSTILNIK S.A., UGRYUMOV A.V., KNIAZEVA T.F., PRAMSKY A.G., BROSCH N., HAGEN H.-J., HOPP U., IZOTOV Y.I., LIPOVETSKY V.A., MASEGOSA J., MARQUEZ I., MARTIN J.-M.
	Astron. Astrophys., 366, 771-787 (2001)
	The Hamburg/SAO survey for emission-line galaxies. IV. The fourth list of 119 galaxies.
o	Tables 3-8: <HS HHMM+DDMMA> N=119.
Ref:	=2001A&A...374..907U
by	UGRYUMOV A.V. , ENGELS D., KNIAZEV A.Y., GREEN R.F., IZOTOV Y.I., HOPP U., PUSTILNIK S.A., PRAMSKY A.G., KNIAZEVA T.F., BROSCH N., HAGEN H.-J., LIPOVETSKY V.A., MASEGOSA J., MARQUEZ I., MARTIN J.-M.
	Astron. Astrophys., 374, 907-913 (2001)
	The Hamburg/SAO survey for emission-line galaxies. V. The fifth list of 161 galaxies.
o	Tables 3-7: <HS HHMM+DDMMA> N=161.
Ref:	=2005A&A...442..109P
by	PUSTILNIK S.A. , ENGELS D., LIPOVETSKY V.A., KNIAZEV A.Y., PRAMSKIJ A.G., UGRYUMOV A.V., MASEGOSA J., IZOTOV Y.I., CHAFFEE F., MARQUEZ I., TEPLYAKOVA A.L., HOPP U., BROSCH N., HAGEN H.-J., MARTIN J.-M.
	Astron. Astrophys., 442, 109-116 (2005)
	The Hamburg/SAO survey for emission-line galaxies. VI. The sixth list of 126 galaxies.
o	Tables 3-7: <HS HHMM+DDMMA> N=126.
=E=	Catalogue in electronic form as J/A+AS/128/507
=E=	Catalogue in electronic form as J/A+AS/135/511
=E=	Catalogue in electronic form as J/A+AS/137/299
=E=	Catalogue in electronic form as J/A+AS/142/417
=E=	Catalogue in electronic form as J/A+A/366/771
=E=	Catalogue in electronic form as J/A+A/374/907
=E=	Catalogue in electronic form as J/A+A/442/109
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HS
HS	(Hodge+Sexton)
Rem:	Identif. charts
*****	Avoid the usage of HS, prefer [HS66]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HS
HS	(Hoag+Smith)
*****	Avoid the usage of HS, prefer [HS77]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HS
HS	(Humphreys+Sandage)
Origin	of the Acronym: L (1998ApJ...505..793M)
Details on Acronym: HS
HS	(Henize, Star)
*****	Avoid the usage of HS, prefer LHA 115-S
Origin	of the Acronym: L (2002ApJS..141...81M)
Details on Acronym: HS
HS	(Henize, Star)
*****	Avoid the usage of HS, prefer LHA 120-S
Origin	of the Acronym: L (2002ApJS..141...81M)
Details on Acronym: HS
HS	(Hot Spot)
*****	Avoid the usage of HS, prefer [LSB2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HS
HS	(Hot Spot)
*****	Avoid the usage of HS, prefer [MRD82]
Origin	of the Acronym: L (1992AJ....104.1525D)
Details on Acronym: [HS2000]
[HS2000]	(Haberl+Sasaki, 2000)= ([HS2000a])
Write:	<<[HS2000] NN>>
N:	60
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	N=60 X-ray sources correlating with em-line objects or identified as High mass X-ray binaries in the SMC.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2000A&A...359..573H
by	HABERL F. , SASAKI M.
	Astron. Astrophys., 359, 573-585 (2000)
	Doubling the number of Be/X-ray binaries in the SMC.
o	in ref list: Inoue 1983IAUS..101..535 instead of p.237
o	Table 1: <[HS2000] NN> (Nos 1-60).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HS2000a]
[HS2000a]	(Haberl+Sasaki, 2000)
*****	Avoid the usage of [HS2000a], prefer [HS2000]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HS2000b]
[HS2000b]	(Howk+Savage, 2000)= (DIG)
Write:	<<[HS2000b] DIG+xxx+yyy>>
N:	7
Object:	Feature (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	Diffuse Ionised Gas (DIG) in NGC 891. '+xxx' is the distance in arcsec from the optical center of the galaxy traced along the major axis, '+yyy' the distance along the minor axis. See also [HS97] and [HS99].
in source:	NGC 891
Ref:	=2000AJ....119..644H
by	HOWK J.C. , SAVAGE B.D.
	Astron. J., 119, 644-667 (2000)
	The multiphase halo of NGC 891: WIYN Hα and BVI imaging.
o	Table 4: <[HS99] NGC 891:+xxx+yyy> N=10 added. Table 6: <[HS2000b] DIG+xxx+yyy> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HS2005]
[HS2005]	(Hota+Saikia, 2005)
Write:	<<[HS2005] JHHMMSS.ss+DDMMSS.s>>
N:	7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	GMRT and VLA observations of NGC 1482. N=7 nuclear emission peaks at different wavelengths.
in source:	NGC 1482
Ref:	=2005MNRAS.356..998H
by	HOTA A. , SAIKIA D.J.
	Mon. Not. R. Astron. Soc., 356, 998-1008 (2005)
	A radio study of the superwind galaxy NGC 1482.
o	Table 4: <[HS2005] JHHMMSS.ss+DDMMSS.s> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HS53]
[HS53]	(Hubble+Sandage, 1953)= (H-S)
Write:	<<[HS53] M 31 Var 19 NN>> <<[HS53] M 33 Center NN>> <<[HS53] M 33 Var A NN>> <<[HS53] A>>
N:	22+33+23+3
Object:	* (SIMBAD class: Star)
Note:	Table 1: Standard stars, N=22 in M 31 region around 'Var 19' (BASW 19), N=33 in M 33 center region, N=23 in M 33 region around [HS53] A. Table 2: three new variable stars: A, B, C, often named H-S stars in the literature.
in source:	M 31 = NGC 224
in source:	M 33 = NGC 598
Ref:	=1953ApJ...118..353H
by	HUBBLE E. , SANDAGE A.
	Astrophys. J., 118, 353-361 (1953)
	The brightest variable stars in extragalactic nebulae. I. M31 and M33.
o	T.1: Var 19 in M 31 = BASW 19. T.2: Star 2 in M 33 = VHK 2.
o	Table 1: <[HS53] M 31 Var 19 NN> (Nos 1-22), <[HS53] M 33 Center NN> (Nos 1-33), <[HS53] M 33 Var A NN> (Nos 1-23). Table 2: <[HS53] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HS66]
[HS66]	(Hodge+Sexton, 1966)= (HS)
Write:	<<[HS66] NNNA>>
N:	455
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Rem:	Identif. charts
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1966AJ.....71..363H
by	HODGE P.W. , SEXTON J.A.
	Astron. J., 71, 363-368 (1966)
	457 New Star Clusters of the Large Magellanic Cloud.
o	Fig 1: The 6 uncatalogued clusters 'U' have no individual designation, they are not in SIMBAD.
o	Table II: <[HS66] NNNA> (Nos 1-455) N=458
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HS75]
[HS75]	(Hodge+Snow, 1975)
Write:	<<[HS75] NN>>
N:	30
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=30 probable SMC bright background galaxies
Ref:	=1975AJ.....80....9H
by	HODGE P.W. , SNOW T.P.
	Astron. J., 80, 9-10 (1975)
	Finding list of bright galaxies behind the SMC.
o	Table I: Atlas ID (Hodge, Suppl. No. 1 to the SMC Atlas) not in SIMBAD
o	Table I: <[HS75] NN> (Nos 1-30)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HS77]
[HS77]	(Hoag+Smith, 1977)= (HS) = (Hoag)
Write:	<<[HS77] HHMMSS.s+DDMMSS>>
N:	76
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Ref:	=1977ApJ...217..362H
by	HOAG A.A. , SMITH M.G.
	Astrophys. J., 217, 362-381 (1977)
	Faint emission-line quasi-stellar object candidates.
o	<[HS77] HHMMSS.s-DDMMSS> N=76
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HS79]
[HS79]	(Hintzen+Scott, 1977)= (HS) (Not yet in Simbad)
Write:	<<[HS79] NNN>>
N:	17
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	N=17 G in ACO 2142 among (Nos 101-402)
in source:	ACO 2142
Ref:	=1979A&A....74..116H
by	HINTZEN P. , SCOTT J.S.
	Astron. Astrophys., 74, 116-117 (1979)
	The X-ray cluster A 2142.
o	<[HS79] NNN> N=17 among (Nos 101-402)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HS80]
[HS80]	(Humphreys+Sandage, 1980)= (HS) = (OB)
Write:	<<[HS80] NNNa>> <<[HS80] TA>> <<[HS80] TNN>> <<[HS80] QNN>> <<[HS80] BNNN a>> <<[HS80] RNNN a>> <<[HS80] NNNaA>>
N:	197+22+13+20+610+412+55
Object:	Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 2: Assoc. format 'NNNa' (Nos 1-143), Assoc. 66a, b and c being triple in the first ref., . This table is continued in the second ref.: (Nos 144-197) ([KI84] use [HS80]). Table 3: formats 'TA', 'TNN' and 'QNN' (N=22, 13 and 20 respectively) for transfer stars. Table 5: format 'BNNN' for Blue stars, N=610. Table 6: format 'RNNN' for Red stars, N=412. Table 7: format 'NNNaA' for stars in the NNNa associations of table 2. Finding chart. See also: [SK76], [S83], [S84b], [S84c], [SC85], [SC85b], [SC86], [SC88], [SCK96], and outside the series: [SC82]
in source:	M 33 = NGC 598
Ref:	=1980ApJS...44..319H
by	HUMPHREYS R.M. , SANDAGE A.
	Astrophys. J., Suppl. Ser., 44, 319-381 (1980)
	On the stellar content and structure of the spiral galaxy M 33.
o	T.2: <[HS80] NNNa> N=143. T.3: <[HS80] TA> N=22, <[HS80] TNN> N=13, <[HS80] QNN> N=20. T. 5: <[HS80] BNNN>, <[HS80] BNNN a> N=610. T.6: <[HS80] RNNN>, <[HS80] RNNN a> N=412. T. 7: <[HS80] NNNaA> N=55
Ref:	=1984Ap&SS.106..371K
by	KUNCHEV P.Z. , IVANOV G.R.
	Astrophys. Space Sci., 106, 371-379 (1984)
	New stellar associations in M 33 galaxy.
o	<[HS80] NNN> (Nos 144-197), [KI84]: use [HS80]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HS83]
[HS83]	(Humphreys+Strom, 1983)
Write:	<<[HS83] NN>>
N:	93
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	M 101 = NGC 5457
Ref:	=1983ApJ...264..458H
by	HUMPHREYS R.M. , STROM S.E.
	Astrophys. J., 264, 458-463 (1983)
	M supergiants and the distance to M 101.
o	<[HS83] NN> N=93
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HS87]
[HS87]	(Hopp+Schulte-Ladbeck, 1987)
Write:	<<[HS87] BRI-NN>> <<[HS87] RI-NN>> <<[HS87] {B\|R\|I}-NNN>>
N:	80+56+46+61+123
Object:	* (SIMBAD class: Star)
Note:	CCD images and spectroscopy of Holmberg IX with Calar Alto 3.5m telescope. Table 1: 'BRI-NN', stars measured in BRI. Table 2: 'RI-NN', stars only measured in RI. Table 3: 'A-NNN', stars measured only in one filter (B, R, or I).
in source:	Holmberg IX
Ref:	=1987A&A...188....5H
by	HOPP U. , SCHULTE-LADBECK R.E.
	Astron. Astrophys., 188, 5-12 (1987)
	The stellar content and morphology of the dwarf irregular galaxy Holmberg IX.
o	Table 1: <[HS87] BRI -NN> (Nos 1-80). Table 2: <[HS87] RI-NN> (Nos 1-56). Table 3: <[HS87] A-NNN> (Nos B-1 to B-46, R-1 to R-61, I-1 to I-123).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HS95]
[HS95]	(Hopp+Schulte-Ladbeck, 1995)
Write:	<<[HS95] UGC NNNN NNN>> <<[HS95] DDO 210 BV NNN>> <<[HS95] DDO 210 VR NNN>>
N:	1689
Object:	* (SIMBAD class: Star)
Note:	Maps fig. 4-12. Table 8: Format 'UGC 4459 NNN', (Nos 1-159) * in UGC 4459. Table 9: Format 'UGC 7559 NNN', (Nos 1-169) * in UGC 7559. Table 10: Format 'UGC 8024 NNN', (Nos 1-210) * in UGC 8024. Table 11: Format 'UGC 8091 NNN', (Nos 1-178) * in UGC 8091. Table 12: Format 'DDO 210 BV NNN', (Nos 1-227), photometry BV, * in DDO 210. Table 13: Format 'DDO 210 VR NNN', (Nos 1-325), photometry VR, * in DDO 210. Table 14: Format 'UGC 5272 NNN', (Nos 1-133) * in UGC 5272. Table 15: Format 'UGC 5340 NN', (Nos 1-77) * in UGC 5340. Table 16: Format 'UGC 6456 NN', (Nos 1-17) * in UGC 6456. Table 17: Format 'UGC 8320 NN', (Nos 1-86) * in UGC 8320. Table 18: Format 'UGC 8760 NNN', (Nos 1-116) * in UGC 8760.
in source:	UGC 4459
in source:	UGC 7559
in source:	UGC 8024
in source:	UGC 8091
in source:	UGC 5272
in source:	UGC 5340
in source:	UGC 6456
in source:	UGC 8320
in source:	UGC 8760
in source:	NAME Aquarius Dwarf Galaxy = DDO 210
Ref:	=1995A&AS..111..527H
by	HOPP U. , SCHULTE-LADBECK R.E.
	Astron. Astrophys., Suppl. Ser., 111, 527-564 (1995)
	CCD photometry of 11 resolved dwarf irregular galaxies.
o	Tables 8 to 11, 14 to 18: <[HS95] UGC NNNN NNN> N=159+169+210+178+133+77+17+86+116. Table 12: <[HS95] DDO 210 BV NNN> N=227, Table 13: <[HS95] DDO 210 VR NNN> N=325
=E=	Catalogue in electronic form as J/A+AS/111/527
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HS96]
[HS96]	(Huang+Sarazin, 1996)
Write:	<<[HS96] A>>
N:	15
Object:	(X) in ClG (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations
in source:	ACO 2151
Ref:	=1996ApJ...461..622H
by	HUANG Z. , SARAZIN C.L.
	Astrophys. J., 461, 622-640 (1996)
	A high-resolution ROSAT X-ray study of the Hercules cluster.
o	Table 1: <[HS96] A> (Nos A-O)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HS97]
[HS97]	(Howk+Savage, 1997)
Write:	<<[HS97] NNa>>
N:	13
Object:	Feature (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	Dust features in NGC 891. See also [HS99].
in source:	NGC 891
Ref:	=1997AJ....114.2463H
by	HOWK J.C. , SAVAGE B.D.
	Astron. J., 114, 2463-2478 (1997)
	Extraplanar dust in the edge-on spiral NGC 891.
o	in ref list: Basu 1997ApJ.480L.55 instead of 480,55
o	Table 2: <[HS97] NNa> (Nos 1-10, 11a-11b, 12)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HS98]
[HS98]	(Huchtmeier+Skillman, 1998)
Write:	<<[HS98] AA>>
N:	2
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
in source:	NAME M 31 GROUP
Ref:	=1998A&AS..127..269H
by	HUCHTMEIER W.K. , SKILLMAN E.D.
	Astron. Astrophys., Suppl. Ser., 127, 269-276 (1998)
	An optically directed HI search for new dwarf members of the M 81 group.
o	Table 1: objects 'NNNA' = [LSK86] NNNA in SIMBAD.
o	Table 1: <[HS98] AA> (Nos OC, OD).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HS99]
[HS99]	(Howk+Savage, 1999)
Write:	<<[HS99] NGC NNNN:D+xxx+yyy>>
N:	22
Object:	Feature (SIMBAD class: Cloud)
Note:	Dust features and filaments in 7 NGC edge-on spiral galaxies. In the format, the letter 'D' stands for Dust cloud, '+xxx' is the distance in arcsec from the optical center of the galaxy traced along the major axis, '+yyy' the distance along the minor axis. See also [HS97] and [HS2000b] for NGC 891.
in source:	NGC 891
in source:	NGC 3628
in source:	NGC 4013
in source:	NGC 4217
in source:	NGC 4302
in source:	NGC 4565
in source:	NGC 4634
Ref:	=1999AJ....117.2077H
by	HOWK J.C. , SAVAGE B.D.
	Astron. J., 117, 2077-2101 (1999)
	A search for extraplanar dust in nearby edge-on spirals.
o	Table 4: <[HS99] NGC NNNN:D+xxx+yyy> N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSB2012]
[HSB2012]	(Hur+Sung+Bessell, 2012)= ([HSB2012a])
Write:	<<[HSB2012] NNNN>>
N:	4543
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Siding Spring Observatory 1m telescope UBVIc photometry of the young open clusters Trumpler 14 and Trumpler 16.
in source:	Cl Trumpler 14
in source:	Cl Trumpler 16
Ref:	=2012AJ....143...41H
by	HUR H. , SUNG H., BESSELL M.S.
	Astron. J., 143, 41 (2012)
	Distance and the initial mass function of young open clusters in the η Carina Nebula: Tr 14 and Tr 16.
o	Table 1: <[HSB2012] NNNN> (Nos 1-4543).
=E=	Catalogue in electronic form as <J/AJ/143/41/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSB2012a]
[HSB2012a]	(Hur+Sung+Bessell, 2012)
*****	Avoid the usage of [HSB2012a], prefer [HSB2012]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSB2012b]
[HSB2012b]	(Hussmann+Stolte+Brandner+, 2012)
Write:	<<[HSB2012b] NNNN>>
N:	1221
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT NAOS/CONICA NIR observations of the Quintet Cluster.
in source:	NAME Quintuplet Cluster
Ref:	=2012A&A...540A..57H
by	HUSSMANN B. , STOLTE A., BRANDNER W., GENNARO M., LIERMANN A.
	Astron. Astrophys., 540A, 57-57 (2012)
	The present-day mass function of the Quintuplet cluster based on proper motion membership.
o	Table 4: <[HSB2012b] NNNN> (Nos 1-1221).
=E=	Catalogue in electronic form as J/A+A/540/A57
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSB2012c]
[HSB2012c]	(Haberl+Sturm+Ballet+, 2012)= (XMMU)
Write:	<<[HSB2012c] XMMU JHHMM.m+DDMM>>
N:	4
Object:	Poss. SNR (SIMBAD class: SNRemnant_Candidate = SuperNova Remnant Candidate)
Stat:	is completely incorporated in Simbad
Note:	XMM EPIC observations of N=3 SNR candidates in the Small Magellanic Cloud.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2012A&A...545A.128H
by	HABERL F. , STURM R., BALLET J., BOMANS D.J., BUCKLEY D.A.H., COE M.J., CORBET R., EHLE M., FILIPOVIC M.D., GILFANOV M., HATZIDIMITRIOU D., LA PALOMBARA N., MEREGHETTI S., PIETSCH W., SNOWDEN S., TIENGO A.
	Astron. Astrophys., 545A, 128-128 (2012)
	The XMM-Newton survey of the Small Magellanic Cloud.
o	Fig. 9, Table 3: XMMU J010834.5-727000 is a misprint for XMMU J010834.5-722700.
o	Fig. 6, Table 2: <[HSB2012c] XMMU JHHMM.m+DDMM> N=4.
=E=	Catalogue in electronic form as J/A+A/545/A128
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HSC
HSC	(Hyper Suprime-Cam) (Not yet in Simbad)
Write:	<<HSC YYaaaa>>
N:	1824
Object:	Poss. SN (SIMBAD class: Supernova_Candidate = SuperNova Candidate)
Note:	N=1824 SN candidates, as part of a deep transient survey of the COSMOS field with the Subaru Hyper Suprime-Cam (HSC).
in source:	NAME COSMOS Field
Ref:	=2019PASJ...71...74Y
by	YASUDA N. , TANAKA M., TOMINAGA N., et al.
	PASJ, 71, 74 (2019)
	The Hyper Suprime-Cam SSP transient survey in COSMOS: Overview.
o	<HSCYYaaaa> N=1824.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HSC
HSC	(Hyper Suprime-Cam)
====>	Equivalent to: HSCS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HSC-SN
HSC-SN	(Subaru/Hyper Suprime-Cam SN)
Write:	<<HSC-SN YYaa>>
N:	81
Object:	Poss. SN (SIMBAD class: Supernova_Candidate = SuperNova Candidate)
Note:	Supernova candidates from a transient survey with Subaru/Hyper Suprime-Cam (HSC).
Ref:	=2014ATel.6291....1T
by	TOMINAGA N. , MOROKUMA T., TANAKA M., YASUDA N., FURUSAWA H., JIANG J., MIYAZAKI S., MORIYA T.J., NOUMARU J., SCHUBERT K., TAKATA T.
	ATel, 6291, 1 (2014)
	First supernova candidates discovered with Subaru/Hyper Suprime-Cam.
o	<HSC-SNYYa> (Nos 14a-14h).
Ref:	=2014ATel.6763....1T
by	TOMINAGA N. , MOROKUMA T., TANAKA M., YASUDA N., FURUSAWA H., JIANG J., OKABE N., FUTAMASE T., MIYAZAKI S., MORIYA T.J., NOUMARU J., SCHUBERT K., TAKATA T.
	ATel, 6763, 1 (2014)
	Supernova candidates discovered with Subaru/Hyper Suprime-Cam.
o	<HSC-SNYYa> (Nos 14i-14u) added.
Ref:	=2015ATel.7565....1T
by	TOMINAGA N. , MOROKUMA T., TANAKA M., JIANG J.-A., KATO T., TANIGUCHI Y., YASUDA N., FURUSAWA H., OKABE N., FUTAMASE T., MIYAZAKI S., MORIYA T.J., NOUMARU J., SCHUBERT K., TAKATA T.
	ATel, 7565, 1 (2015)
	Fifty supernova candidates discovered with Subaru/Hyper Suprime-Cam.
o	<HSC-SNYYaa> (Nos 15a-15z, 15aa-15ax) added.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HSC2004]
[HSC2004]	(Hiriart+Salas+Cruz-Gonzalez, 2004) (Not yet in Simbad)
Write:	<<[HSC2004] A>>
N:	13
Object:	H2 (SIMBAD class: PartofCloud = Part of Cloud)
Note:	Structure of molecular hydrogen outflow associated with the star-forming region Cep A. Regions (B to G) are in Cep A East, (H to M) in Cep A West.
in source:	NAME Cep A
Ref:	=2004AJ....128.2917H
by	HIRIART D. , SALAS L., CRUZ-GONZALEZ I.
	Astron. J., 128, 2917-2931 (2004)
	Molecular hydrogen kinematics in Cepheus A.
o	Fig.9, Table 1: <[HSC2004] A> (Nos B-M).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSC2011]
[HSC2011]	(Hill+Szostek+Corbel+, 2011)
Write:	<<[HSC2011] JHHMMSS+DDMMSS W>>
N:	5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA, GMRT, Parkes and VLT radio continuum observations of the field of 1FGL J1227.9-4852.
Ref:	=2011MNRAS.415..235H
by	HILL A.B. , SZOSTEK A., CORBEL S., CAMILO F., CORBET R.H.D., DUBOIS R., DUBUS G., EDWARDS P.G., FERRARA E.C., KERR M., KOERDING E., KOZIEL D., STAWARZ L.
	Mon. Not. R. Astron. Soc., 415, 235-243 (2011)
	The bright unidentified γ-ray source 1FGL J1227.9-4852: can it be associated with a low-mass X-ray binary?
o	Fig. 4, Paragr. 2.2: <[HSC2011] JHHMMSS+DDMMSSW> N=5.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSC96]
[HSC96]	(High-z supernova search team+Suntzeff+Clocchiatti+, 1996)
Write:	<<[HSC96] JHHMMSS.ss+DDMMSS.s>>
N:	17
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxies of SN 1996AT to SN 1996BJ.
Ref:	=1996IAUC.6490....1H
by	HIGH-Z SUPERNOVA SEARCH TEAM , SUNTZEFF N., CLOCCHIATTI A., SCHOMMER R., SCHMIDT B., STATHAKIS R., FILIPPENKO A.V., LEONARD D.C., BARTH A.J., KIRSHNER R.
	IAU Circ., 6490, 1-None (1996)
	Supernovae.
o	(Erratum) + corrigendum IAUC 6491
o	<[HSC96] JHHMMSS.ss+DDMMSS.s> N=17.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HSCS
HSCS	(Hyper Suprime-Cam Survey)= HSC
Write:	<<HSCS JHHMMSS+DDMMSS>> <<HSCS JHHMMSS.ss+DDMMSS.s>>
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Hyper Suprime-Cam Subaru Strategic Survey is a three-layered, multi-band (grizy plus 4 narrow-band filters) imaging survey with the Hyper Suprime-Cam (HSC) on the 8.2m Subaru Telescope. For more information, visit: http://hsc.mtk.nao.ac.jp/ssp/survey/ and also https://hsc-release.mtk.nao.ac.jp/ for the data releases.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HSCv1
HSCv1	(Hubble Source Catalog version 1)
Write:	<<HSCv1 NNNNNNNN>>
N:	32109825
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	The Hubble Source Catalog (HSC) is designed to optimize science from the Hubble Space Telescope by combining the tens of thousands of visit-based source lists in the Hubble Legacy Archive (HLA) into a single master catalog. Please, note that the numbering (col. MatchID) changes between the versions. For more information, visit the HSCv1 MAST webpage (https://archive.stsci.edu/hst/hscv1/) and the HLA (https://hla.stsci.edu/) webpage. See also HSCv2, HSCv3.
Ref:	=2016AJ....151..134W
by	WHITMORE B.C. , ALLAM S.S., BUDAVARI T., CASERTANO S., DOWNES R.A., DONALDSON T., FALL S.M., LUBOW S.H., QUICK L., STROLGER L.-G., WALLACE G., WHITE R.L.
	Astron. J., 151, 134-134 (2016)
	Version 1 of the Hubble Source Catalog.
o	<HSCv1 NNNNNNNNNN> (Nos 1-32109825).
=E=	Catalogue in electronic form as <II/342/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HSCv2
HSCv2	(Hubble Source Catalog version 2)
Write:	<<HSCv2 NNNNNNNN>>
N:	32109825
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	The Hubble Source Catalog (HSC) is designed to optimize science from the Hubble Space Telescope by combining the tens of thousands of visit-based source lists in the Hubble Legacy Archive (HLA) into a single master catalog. Please, note that the numbering (col. MatchID) changes between the versions. For more information, visit the HSCv2 MAST webpage (https://archive.stsci.edu/hst/hscv2/) and the HLA (https://hla.stsci.edu/) webpage. See also HSCv1, HSCv3.
=E=	Catalogue in electronic form as <II/342/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HSCv3
HSCv3	(Hubble Source Catalog version 3)
Write:	<<HSCv3 NNNNNNNN>>
N:	32109825
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	The Hubble Source Catalog (HSC) is designed to optimize science from the Hubble Space Telescope by combining the tens of thousands of visit-based source lists in the Hubble Legacy Archive (HLA) into a single master catalog. Please, note that the numbering (col. MatchID) changes between the versions. For more information, visit the HSCv3 MAST webpage (https://archive.stsci.edu/hst/hsc/) and the HLA (https://hla.stsci.edu/) webpage. See also HSCv1, HSCv2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HSD
HSD	(Hoessel+Schommer+Danielson) (Not yet in Simbad)
*****	Avoid the usage of HSD, prefer [HSD83]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HSD2007]
[HSD2007]	(Hao+Stanek+Dobrzycki+, 2007) (Not yet in Simbad)
Write:	<<[HSD2007] GRB 060206 abs N.NN>>
N:	1
Object:	Absorber
Note:	Absorption lines in the spectra of GRB 060206. See also [FLC2006b] and [FSL2006].
Ref:	=2007ApJ...659L..99H
by	HAO H. , STANEK K.Z., DOBRZYCKI A., MATHESON T., BENTZ M.C., KURASZKIEWICZ J., GARNAVICH P.M., HOWK J.C., CALKINS M.L., WORTHEY G., MODJAZ M., SERVEN J.
	Astrophys. J., 659L, 99-102 (2007)
	Strongly variable z=1.48 Fe II and Mg II absorption in the spectra of z=4.05 GRB 060206.
o	Fig.1: <[HSD2007] GRB 060206 abs N.NN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSD83]
[HSD83]	(Hoessel+Schommer+Danielson, 1983)= (HSD) (Not yet in Simbad)
Write:	<<[HSD83] NNN>>
N:	652
Object:	* (SIMBAD class: Star)
Note:	See also: [HM82], [HD83], [HD84], [HA86]
in source:	Sextans A = DDO 75
Ref:	=1983ApJ...274..577H
by	HOESSEL J.G. , SCHOMMER R.A., DANIELSON G.E.
	Astrophys. J., 274, 577-594 (1983)
	Photometry of resolved galaxies. II. Sextans A.
o	Table 1: objects are not in SIMBAD
o	Table 1: <[HSD83] NNN> (Nos 100-751)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSD93a]
[HSD93a]	(Heithausen+Stacy +De Vries+, 1993)
*****	Avoid the usage of [HSD93a], prefer HSVMT
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSD93b]
[HSD93b]	(Hu+Slijkhuis+De Jong+, 1993)
Write:	<<[HSD93b] NN>>
N:	62
Object:	Poss. proto-PN (SIMBAD class: post-AGB*_Candidate = Post-AGB Star Candidate)
Stat:	is completely incorporated in Simbad
Ref:	=1993A&AS..100..413H
by	HU J.Y. , SLIJKHUIS S., DE JONG T., JIANG B.W.
	Astron. Astrophys., Suppl. Ser., 100, 413-430 (1993)
	A systematic study of IRAS selected proto-planetary nebula candidates. I. Selection of a sample and obervations of the southern objects.
o	Table 3: <[HSD93b] NN> N=62
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSD93c]
[HSD93c]	(Howell+Schmidt+DeYoung+, 1993) (Not yet in Simbad)
Write:	<<[HSD93c] NN>>
N:	6
Object:	* (SIMBAD class: Star)
Note:	Comparison stars in the field of EF Peg. See also [TGS79].
Ref:	=1993PASP..105..579H
by	HOWELL S.B. , SCHMIDT R., DE YOUNG J.A., FRIED R., SCHMEER P., GRITZ L.
	Publ. Astron. Soc. Pac., 105, 579-585 (1993)
	Photometry of EF Pegasi during superoutburst.
o	Fig.1, Table 4: stars format 'a' = [TGS79] a in SIMBAD
o	Fig.1, Table 4: <[HSD93c] N> (Nos 5-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSD98]
[HSD98]	(Hughes+Serjeant+Dunlop+, 1998)= (HDF) = (HDF850) = ([HSD98a])
Write:	<<[HSD98] HDF850.N>>
N:	8
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	Deep submillimeter survey in the HDF, at 850microm.
in source:	NAME HDFN
Ref:	=1998Natur.394..241H
by	HUGHES D.H. , SERJEANT S., DUNLOP J., ROWAN-ROBINSON M., BLAIN A., MANN R.G., IVISON R., PEACOCK J., EFSTATHIOU A., GEAR W., OLIVER S., LAWRENCE A., LONGAIR M., GOLDSCHMIDT P., JENNESS T.
	Nature, 394, 241-247 (1998)
	High-redshift star formation in the Hubble Deep Field revealed by a submillimetre-wavelength survey.
o	Table 1: <[HSD98] HDF850.N> (Nos 1-5)
Ref:	=2003MNRAS.344..887S
by	SERJEANT S. , DUNLOP J.S., MANN R.G., ROWAN-ROBINSON M., HUGHES D., EFSTATHIOU A., BLAIN A., FOX M., IVISON R.J., JENNESS T., LAWRENCE A., LONGAIR M., OLIVER S., PEACOCK J.A.
	Mon. Not. R. Astron. Soc., 344, 887-904 (2003)
	Submillimetre observations of the Hubble Deep Field and Flanking Fields.
o	Fig.7: galaxies 'NNNNN NNNN' are 'HDFFF MMSSs-MMSS' in SIMBAD.
o	Table 1: <[HSD98] HDF850.N> (Nos 6-8) added.
=E=	Catalogue in electronic form as J/MNRAS/344/887
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSD98a]
[HSD98a]	(Hughes+Serjeant+Dunlop+, 1998) F HDF850.N
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
in source:	NAME HDFN
Ref:	=1998Natur.394..241H
by	HUGHES D.H. , SERJEANT S., DUNLOP J., ROWAN-ROBINSON M., BLAIN A., MANN R.G., IVISON R., PEACOCK J., EFSTATHIOU A., GEAR W., OLIVER S., LAWRENCE A., LONGAIR M., GOLDSCHMIDT P., JENNESS T.
	Nature, 394, 241-247 (1998)
	High-redshift star formation in the Hubble Deep Field revealed by a submillimetre-wavelength survey.
o	Table 1: <[HSD98] HDF850.N> (Nos 1-5)
Ref:	=2003MNRAS.344..887S
by	SERJEANT S. , DUNLOP J.S., MANN R.G., ROWAN-ROBINSON M., HUGHES D., EFSTATHIOU A., BLAIN A., FOX M., IVISON R.J., JENNESS T., LAWRENCE A., LONGAIR M., OLIVER S., PEACOCK J.A.
	Mon. Not. R. Astron. Soc., 344, 887-904 (2003)
	Submillimetre observations of the Hubble Deep Field and Flanking Fields.
o	Fig.7: galaxies 'NNNNN NNNN' are 'HDFFF MMSSs-MMSS' in SIMBAD.
o	Table 1: <[HSD98] HDF850.N> (Nos 6-8) added.
*****	Avoid the usage of [HSD98a], prefer [HSD98]
=E=	Catalogue in electronic form as J/MNRAS/344/887
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSD98b]
[HSD98b]	(Hoessel+Saha+Danielson, 1998)= [HSD98b] (Not yet in Simbad)
Write:	<<[HSD98b] Ho II VNN>> <<[HSD98b] DDO 187 VNN>>
N:	28+12
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Maps See also [TSH95], [SHK96]
in source:	Holmberg II = DDO 50
Ref:	=1998AJ....115..573H
by	HOESSEL J.G. , SAHA A., DANIELSON G.E.
	Astron. J., 115, 573-583 (1998)
	Variable stars in the Holmberg II dwarf galaxy.
o	Table 3: <[HSD98b] Ho II VNN> (Nos V1-V28).
Ref:	=1998AJ....116.1679H
by	HOESSEL J.G. , SAHA A., DANIELSON G.E.
	Astron. J., 116, 1679-1687 (1998)
	Variable stars in the DDO 187 dwarf galaxy.
o	Table 2: <[HSD98] DDO 187 VNN> (Nos V1-V12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: hSDF
hSDF	(host, SDF)
====>	Equivalent to: [GPM2011]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: hSDF
hSDF	(host, SDF)
Write:	<<hSDF YYMM.NN>>
N:	31
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck LRIS and DEIMOS spectroscopy. Subaru telescope observations of the SDF to search for supernovae (see SNSDF) and their host galaxies. See [GPM2011] for additional supernovae and host galaxies. See also [PMY2007].
in source:	NAME SDF
Ref:	=2007MNRAS.382.1169P
by	POZNANSKI D. , MAOZ D., YASUDA N., FOLEY R.J., DOI M., FILIPPENKO A.V., FUKUGITA M., GAL-YAM A., JANNUZI B.T., MOROKUMA T., ODA T., SCHWEIKER H., SHARON K., SILVERMAN J.M., TOTANI T.
	Mon. Not. R. Astron. Soc., 382, 1169-1186 (2007)
	Supernovae in the Subaru Deep Field: an initial sample and Type Ia rate out to redshift 1.6.
o	Table 1: <SNSDF YYMM.NN> N=33. Table 2: <hSDF YYMM.NN> N=31. Table 3: <[PMY2007] NNN> (Nos 1-123).
=E=	Catalogue in electronic form as J/MNRAS/382/1169
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HSE2005]
[HSE2005]	(Howell+Sullivan+Ellis, 2005)
Write:	<<[HSE2005] JHHMMSS.ss+DDMMSS.ss>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of SN 2005KY.
Ref:	=2005IAUC.8636....3H
by	HOWELL D.A. , (The Supernova Legacy Survey), SULLIVAN M., ELLIS R.S.
	IAU Circ., 8636, 3-None (2005)
	Supernova 2005ky.
o	<[HSE2005] JHHMMSS.ss+DDMMSS.ss> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSE2008]
[HSE2008]	(Hempel+Schaerer+Egami+, 2008)
Write:	<<[HSE2008] ACO 1835 NNNN>> <<[HSE2008] AC 114 NNNN>>
N:	11+9
Object:	Extremely Red Obj. (SIMBAD class: Galaxy)
Note:	HST ACS, VLT ISAAC, and Spitzer MIPS and IRAC observations of ACO 1835 and ACCG 114. Use of archival CFHT data.
in source:	ACO 1835
in source:	ACCG 114 = ACO S 1077
Ref:	=2008A&A...477...55H
by	HEMPEL A. , SCHAERER D., EGAMI E., PELLO R., WISE M., RICHARD J., LE BORGNE J.-F., KNEIB J.-P.
	Astron. Astrophys., 477, 55-66 (2008)
	EROs found behind lensing clusters. II. Empirical properties, classification, and SED modelling based on multi-wavelength observations.
o	Fig.1, Table 2: <[HSE2008] ACO 1835 NNNN> N=11 among (Nos 305-1093). Fig.2, Table 3: <[HSE2008] AC 114 NNNN> N=9 among (Nos 512-1167).
=E=	Catalogue in electronic form as J/A+A/477/55
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSE2011]
[HSE2011]	(Hart+Stocke+Evrard+, 2011)
Write:	<<[HSE2011] MSHHMM-RN>> <<[HSE2011] RXJHHMM-RN>> <<[HSE2011] MSHHMM-XN>> <<[HSE2011] RXJHHMM-XNN>>
N:	4+22+6+80
Object:	(Rad) + (X) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	VLA 1.4GHz observations and archival Chandra X-ray observations of N=26+86 radio and X-ray sources in 12 high-redshift clusters of galaxies.
Ref:	=2011ApJ...740...59H
by	HART Q.N. , STOCKE J.T., EVRARD A.E., ELLINGSON E.E., BARKHOUSE W.A.
	Astrophys. J., 740, 59 (2011)
	The evolution of radio galaxies and X-ray point sources in Coma cluster progenitors since z ~ 1.2.
o	Table 5: <[HSE2011] MS1621-RN> (Nos R1-R4), <[HSE2011] RXJHHMM-RN> N=22. Table 11: <[HSE2011] MSHHMM-XN> N=6, <[HSE2011] RXJHHMM-XNN> N=80.
=E=	Catalogue in electronic form as J/ApJ/740/59
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSE84]
[HSE84]	(Hummel+Sancisi+Ekers, 1984)
Write:	<<[HSE84] HHMMSS.ss+DDMMSS.s>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=2 radio components of NGC 5907, identical to [DKW2000] sources.
in source:	NGC 5907
Ref:	=1984A&A...133....1H
by	HUMMEL E. , SANCISI R., EKERS R.D.
	Astron. Astrophys., 133, 1-10 (1984)
	Radio continuum observations of the edge-on spiral galaxies NGC 4244, 4565, and 5907.
o	<[HSE84] HHMMSS.ss+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSF2009]
[HSF2009]	(Hau+Spitler+Forbes+, 2009)= (SUCD)
Write:	<<[HSF2009] SUCDN>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST ACS images and Keck DEIMOS spectroscopy of the field of the Sombrero galaxy.
Ref:	=2009MNRAS.394L..97H
by	HAU G.K.T. , SPITLER L.R., FORBES D.A., PROCTOR R.N., STRADER J., MENDEL J.T., BRODIE J.P., HARRIS W.E.
	Mon. Not. R. Astron. Soc., 394L, 97-101 (2009)
	An ultra-compact dwarf around the Sombrero galaxy (M104): the nearest massive UCD.
o	<[HSF2009] SUCD1>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSG2002]
[HSG2002]	(Holland+Soszynski+Gladders+, 2002)
Write:	<<[HSG2002] SN>>
N:	8
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Standard stars in the field of GRB 011211.
Ref:	=2002AJ....124..639H
by	HOLLAND S.T. , SOSZYNSKI I., GLADDERS M.D., BARRIENTOS L.F., BERLIND P., BERSIER D., GARNAVICH P.M., JHA S., STANEK K.Z.
	Astron. J., 124, 639-645 (2002)
	The optical afterglow of the γ-ray burst GRB 011211.
o	Fig.1, Table 2: <[HSG2002] SN> (Nos S0-S7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSG2015]
[HSG2015]	(Hummel+Stanke+Galvan-Madrid+, 2015)
Write:	<<[HSG2015] Sa>> <<[HSG2015] SN>>
N:	7
Object:	Core (SIMBAD class: denseCore = Dense Core)
Note:	APEX SABOCA 350µm continuum observations of N=7 massive cores in the giant HII region NGC 3603.
in source:	NGC 3603
Ref:	=2015A&A...582A..66H
by	HUMMEL C.A. , STANKE T., GALVAN-MADRID R., KORIBALSKI B.S.
	Astron. Astrophys., 582A, 66-66 (2015)
	Massive envelopes and filaments in the NGC 3603 star forming region.
o	Calibrator PKS 1045-62 not identified. B13134 is IRAS 13134-6242.
o	Table 2, Fig. 4: <[HSG2015] Sa> N=5 among (Nos Sa-Sg), <[HSG2015] SN> (Nos S8-S9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSG2019]
[HSG2019]	(Humphreys+Stangl+Gordon+, 2019)
Write:	<<[HSG2019] 10182-p2-22>> <<[HSG2019] 10182-pr-NN>> <<[HSG2019] 10402-7>> <<[HSG2019] 10579-x1-N>> <<[HSG2019] 10584-NN.N>>
N:	1+6+1+3+31
Object:	Poss. V* + HII (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	MMT Hectospec spectroscopy of N=11+31 variable star candidates in NGC 2403 and in M 81 respectively. Use of Hubble Legacy Archive ACS images in the ANGRRR and ANGST programs (proposals GO-10182, GO-10579, GO-10584).
in source:	NGC 2403
in source:	NGC 3031 = M 81
Ref:	=2019AJ....157...22H
by	HUMPHREYS R.M. , STANGL S., GORDON M.S., DAVIDSON K., GRAMMER S.H.
	Astron. J., 157, 22-22 (2019)
	Luminous and variable stars in NGC 2403 and M81.
o	Tables 2+3+7: <[HSG2019] 10182-p2-22> N=1, <[HSG2019] 10182-pr-NN> N=6, <[HSG2019] 10402-7> N=1, <[HSG2019] 10579-x1-N> N=3, <[HSG2019] 10584-NN.N> N=31.
=E=	Catalogue in electronic form as J/AJ/157/22
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSG97]
[HSG97]	(High-z supernova search team+Schmidt+Germany+, 1997)
Write:	<<[HSG97] JHHMMSS.ss+DDMMSS.s>>
N:	19
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxies of SN 1997AS to to 1997BK.
Ref:	=1997IAUC.6602....1H
by	HIGH-Z SUPERNOVA SEARCH TEAM , SCHMIDT B., GERMANY L., SUNTZEFF N., SCHOMMER R., CLOCCHIATTI A., PHILLIPS M., DIERCKS A.
	IAU Circ., 6602, 1-None (1997)
	Supernovae.
o	<[HSG97] JHHMMSS.ss+DDMMSS.s> N=19.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HSGP
HSGP	(Hawkins, South Gal. Pole)= (SGP)
Write:	<<HSGP NN>>
Object:	* (SIMBAD class: Star)
Note:	Hawkins, 1990 private communication. Cited in 1994MNRAS.267...77F and 1995A&AS..109..171F
Auth.:	HAWKINS M.R.S.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HSH2003]
[HSH2003]	(Holt+Schlegel+Hwang+, 2003)
Write:	<<[HSH2003] NN>>
N:	72
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of NGC 6946.
in source:	NGC 6946
Ref:	=2003ApJ...588..792H
by	HOLT S.S. , SCHLEGEL E.M., HWANG U., PETRE R.
	Astrophys. J., 588, 792-800 (2003)
	Chandra observation of the X-ray source population of NGC 6946.
o	Table 1: <[HSH2003] NN> (Nos 1-72).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSH2004]
[HSH2004]	(Hoffman+Salpeter+Hirani, 2004)
Write:	<<[HSH2004] WvW 479 min N>> <<[HSH2004] LMPU NNN+VVV>> <<[HSH2004] LMPU NNN-OFF+VVV>>
N:	2+10+2
Object:	Mini HVC (SIMBAD class: HVCld = High-velocity Cloud)
Stat:	is completely incorporated in Simbad
Note:	Arecibo HI observations of small HVCs.
in source:	WV 479
in source:	LMPU 25
in source:	LMPU 236
in source:	LMPU 387
Ref:	=2004AJ....128.2932H
by	HOFFMAN G.L. , SALPETER E.E., HIRANI A.
	Astron. J., 128, 2932-2941 (2004)
	Mini high-velocity clouds.
o	Table 1: <[HSH2004] WvW 479 min N> (Nos 1-2), <[HSH2004] LMPU NNN+VVV> N=10, <[HSH2004] LMPU NNN-OFF+VVV> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSH2007]
[HSH2007]	(Hall+Sadavoy+Hutsemekers+, 2007) (Not yet in Simbad)
Write:	<<[HSH2007] QSO J0242+0049 abs N.NNNN>> <<[HSH2007] QSO J0242+0049 abs N.NNNNN>>
N:	7
Object:	Absorber
Note:	UVES on the VLT UT2 observations of SDSS J024221.87+004912.6 = QSO J0242+0049.
Ref:	=2007ApJ...665..174H
by	HALL P.B. , SADAVOY S.I., HUTSEMEKERS D., EVERETT J.E., RAFIEE A.
	Astrophys. J., 665, 174-186 (2007)
	Acceleration and substructure constraints in a quasar outflow.
o	<[HSH2007] QSO J0242+0049 abs N.NNNN>, <[HSH2007] QSO J0242+0049 abs N.NNNNN>, N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSH2009]
[HSH2009]	(Hart+Stocke+Hallman, 2009)
Write:	<<[HSH2009] ANNN-XN>> <<[HSH2009] MSHHMM-XN>> <<[HSH2009] A1758-BCG>> <<[HSH2009] RXJHHMM-XN>> <<[HSH2009] ANNNN-RN>> <<[HSH2009] MSHHMM-RN>> <<[HSH2009] RXJHHMM-RN>>
N:	8+20
Object:	(X) + rG (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Use of Chandra archival observations to identify X-ray point sources in clusters of galaxies. VLA 1.4GHz observations of radio galaxies in the same clusters of galaxies.
Ref:	=2009ApJ...705..854H
by	HART Q.N. , STOCKE J.T., HALLMAN E.J.
	Astrophys. J., 705, 854-867 (2009)
	X-ray point sources and radio galaxies in clusters of galaxies.
o	Table 2: <[HSH2009] ANNN-XN>, <[HSH2009] MSHHMM-XN>, <[HSH2009] A1758-BCG>, <[HSH2009] RXJHHMM-XN>, N=8. Table 3: <[HSH2009] ANNNN-RN>, <[HSH2009] MSHHMM-RN>, <[HSH2009] RXJHHMM-RN>, N=20.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSH2012]
[HSH2012]	(Hui+Seo+Huang+, 2012)
Write:	<<[HSH2012] NN>>
N:	17
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS observations of N=17 X-ray sources in the field of G308.3-1.4.
in source:	SNR G308.3-01.4
Ref:	=2012ApJ...750....7H
by	HUI C.Y. , SEO K.A., HUANG R.H.H., TREPL L., WOO Y.J., LU T.-N., KONG A.K.H., WALTER F.M.
	Astrophys. J., 750, 7 (2012)
	Identification campaign of supernova remnant candidates in the Milky Way. I. Chandra observation of G308.3-1.4.
o	Table 1: <[HSH2012] NN> N=17.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSH95]
[HSH95]	(Hunter+Shaya+Holtzman+, 1995)
Write:	<<[HSH95] NNNN>>
N:	3623+26
Object:	* (SIMBAD class: Star)
Note:	1st ref.: Observations from the HST PC2, (Nos 1-3623). 2nd ref.: Observations from the ESO COME ON+. In the 2nd ref., table 2: 1st col. 'NNNN' are [HSH95] numbers, numbers > 9000 are previously unknown sources, N=26. See also [HBO96] and [HBO96b]
in source:	Magellanci Clouds:LMC:RMC 136 = RMC 136
Ref:	=1995ApJ...448..179H
by	HUNTER D.A. , SHAYA E.J., HOLTZMAN J.A., LIGHT R.M., O'NEIL E.J., LYNDS R.
	Astrophys. J., 448, 179-194 (1995)
	The intermediate stellar mass population in R136 determined from Hubble Space Telescope planetary camera 2 images.
o	Table 2 not in SIMBAD
o	Table 2: <[HSH95] NNNN> N=3623
Ref:	=1996ApJ...466..254B
by	BRANDL B. , SAMS B.J., BERTOLDI F., ECKART A., GENZEL R., DRAPATZ S., HOFMANN R., LOEWE M., QUIRRENBACH A.
	Astrophys. J., 466, 254-273 (1996)
	Adaptive optics near-infrared imaging of R136 in 30 Doradus: the stellar population of a nearby starburst.
o	Tables 2, 3 (N=110+971 [HST95] objects) not in SIMBAD
o	Table 2: <[HSH95] 9NNN> N=26 new objects.
=E=	Catalogue in electronic form as J/ApJ/448/179
=E=	Catalogue in electronic form as J/ApJ/466/254
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSH97]
[HSH97]	(Hambly+Smartt+Hodgkin, 1997)
Write:	<<[HSH97] WD 0346+246>>
N:	1
Object:	WD* (SIMBAD class: WhiteDwarf = White Dwarf)
Note:	Serendipitous discovery of a new, very low luminosity, cool degenerate in the region of Taurus. In the format coordinates '0346+246' are neither 1950 coord. (WD 0343+247), nor 2000 coord. (WD J0346+249).
Ref:	=1997ApJ...489L.157H
by	HAMBLY N.C. , SMARTT S.J., HODGKIN S.T.
	Astrophys. J., 489, 157-160 (1997)
	WD 0346+246: a very low luminosity, cool ° in Taurus.
o	Improperly named WD 0346+246 (J2000) instead of WD 0343+247 (B1950)
o	<[HSH97] WD 0346+246> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSJ92]
[HSJ92]	(Hyland+Straw+Jones+, 1992)
Write:	<<[HSJ92] PN>>
N:	4
Object:	Protostar (SIMBAD class: YSO = Young Stellar Object)
Note:	N=4 candidate protostars. See also Dor.
in source:	Magellanic Clouds:LMC:30 Dor Nebula = 30 Dor Nebula
Ref:	=1992MNRAS.257..391H
by	HYLAND A.R. , STRAW S., JONES T.J., GATLEY I.
	Mon. Not. R. Astron. Soc., 257, 391-403 (1992)
	Star formation in the Magellanic Clouds. IV. Protostars in the vicinity of 30 Doradus.
o	Table 2: <Dor IRS NNN> (Nos 1-175). Table 3: <[HSJ92] PN> (Nos P1-P4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HSJG
HSJG	(Hyland+Straw+Jones+Gatley)
*****	Avoid the usage of HSJG, prefer Dor
Origin	of the Acronym: L (2000AJ....119..787G)
Details on Acronym: HSK
HSK	(Hodge+Strobel+Kennicutt)= ([HSK94b])
Write:	<<HSK NN>>
N:	82
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
in source:	Holmberg II = DDO 50
Ref:	=1994PASP..106..309H
by	HODGE P. , STROBEL N.V., KENNICUTT R.C.
	Publ. Astron. Soc. Pac., 106, 309-314 (1994)
	The HII regions of Holmberg II.
o	<HSK NN> N=82
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HSK88]
[HSK88]	(Hummel+Schalinski+Krichbaum+, 1988) (Not yet in Simbad)
Write:	<<[HSK88] 0153+74 A>> <<[HSK88] 0153+74 AN>>
N:	5+7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Radio components of QSO 0153+744.
in source:	QSO B0153+744
Ref:	=1988A&A...204...68H
by	HUMMEL C.A. , SCHALINSKI C.J., KRICHBAUM T.P., WITZEL A., JOHNSTON K.J.
	Astron. Astrophys., 204, 68-72 (1988)
	The quasar 0153+74.
o	<[HSK88] 0153+74 A> (Nos A-D).
Ref:	=1997A&A...324..857H
by	HUMMEL C.A. , KRICHBAUM T.P., WITZEL A., WUELLNER K.H., STEFFEN W., ALEF W., FEY A.
	Astron. Astrophys., 324, 857-869 (1997)
	The radio jet of quasar 0153+744.
o	p.868 : MG 1131-0456 misprint for 1131+0456 = MITG J1131+0456
o	<[HSK88] 0153+74 AN> (Nos E, B1-B3, A1-A4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSK92]
[HSK92]	(Hummel+Schalinski+Krichbaum+, 1988)= (H92)
Write:	<<[HSK92] 1928+738 AN>>
N:	5+4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLBI components of QSO 1928+738. See also [JSE87], [GMR98b], [GMP2000].
in source:	QSO B1928+738
Ref:	=1992A&A...257..489H
by	HUMMEL C.A. , SCHALINSKI C.J., KRICHBAUM T.P., RIOJA M.J., QUIRRENBACH A., WITZEL A., MUXLOW T.W.B., JOHNSTON K.J., MATVEYENKO L.I., SHEVCHENKO A.
	Astron. Astrophys., 257, 489-500 (1992)
	The jets of quasar 1928+738: superluminal motion and large-scale structure.
o	Fig.1, T.1: (Nos 1-7) = [JSE87] 1928+738 1 to 7.
o	Table 3: <[HSK92] 1928+738 AN> (Nos A-E, A1-A2).
Ref:	=1999A&A...348..381R
by	ROS E. , MARCAIDE J.M., GUIRADO J.C., RATNER M.I., SHAPIRO I.I., KRICHBAUM T.P., WITZEL A., PRESTON R.A.
	Astron. Astrophys., 348, 381-393 (1999)
	High precision difference astrometry applied to the triplet of S5 radio sources B1803+784/Q1928+738/B2007+777.
o	Fig.8, Table 6: <[HSK92] 1928+738 AN> (Nos A0, A3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSK94]
[HSK94]	(Hoessel+Saha+Krist+, 1994)= ([HSK94a])
Write:	<<[HSK94] VNN>>
N:	14
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
in source:	DDO 69
Ref:	=1994AJ....108..645H
by	HOESSEL J.G. , SAHA A., KRIST J., DANIELSON G.E.
	Astron. J., 108, 645-652 (1994)
	Variable stars in the Leo A dwarf galaxy (DDO 69).
o	<[HSK94] VNN> N=14
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSK94a]
[HSK94a]	(Hoessel+Saha+Krist+, 1994)
*****	Avoid the usage of [HSK94a], prefer [HSK94]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSK94b]
[HSK94b]	(Hodge+Strobel+Kennicutt, 1994)
*****	Avoid the usage of [HSK94b], prefer HSK
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSL2000]
[HSL2000]	(Henning+Schreyer+Launhardt+, 2000)
Write:	<<[HSL2000] IRS N>> <<[HSL2000] Star A>>
N:	2+2
Object:	(IR) + * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Tables 4, 6: N=2 FIR peaks in IRAS 12091-6129, and N=2 USNO-A2.0 stars in the field. Map Fig.6a.
in source:	IRAS 12091-6129
Ref:	=2000A&A...353..211H
by	HENNING T. , SCHREYER K., LAUNHARDT R., BURKERT A.
	Astron. Astrophys., 353, 211-226 (2000)
	Massive young stellar objects with molecular outflows.
o	Tables 4, 6: <[HSL2000] IRS N> (Nos 1-2), <[HSL2000] Star A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSL2004]
[HSL2004]	(Haas+Siebenmorgen+Leipdki+, 2004)
Write:	<<[HSL2004] JHHMMSS.s+DDMMSS>>
N:	1
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	ISOCAM observations, one ISOCP (ISOCAM Parallel survey) excess source is observed. See also ISOCP.
Ref:	=2004A&A...419L..49H
by	HAAS M. , SIEBENMORGEN R., LEIPSKI C., OTT S., CUNOW B., MEUSINGER H., MUELLER S.A.H., CHINI R., SCHARTEL N.
	Astron. Astrophys., 419, 49-53 (2004)
	Mid-infrared selection of AGN.
o	Fig.2: <ISOCP NNNNN> N=3. Text: <[HSL2004] JHHMMSS.s+DDMMSS> N=1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSM2001]
[HSM2001]	(Hall+Sawicki+Martini+, 2001)
Write:	<<[HSM2001] HHMM+DDd HAN>> <<[HSM2001] HHMM+DDd SMN>> <<[HSM2001] HHMM+DDd NNN>>
N:	5+5+44
Object:	Em* + (submm) + ? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=5 H-alpha emitter candidates in 3 QSOs fields. Table 3: N=5 smm sources in 2 QSOs fields. Table 4: optical-NIR objects in 2 QSOs fields.
Ref:	=2001AJ....121.1840H
by	HALL P.B. , SAWICKI M., MARTINI P., FINN R.A., PRITCHET C.J., OSMER P.S., McCARTHY D.W., EVANS A.S., LIN H., HARTWICK F.D.A.
	Astron. J., 121, 1840-1862 (2001)
	Galaxies in the fields of z~1.5 radio-loud quasars.
o	Table 2: <[HSM2001] HHMM+DDd HAN> N=5. Table 3: <[HSM2001] HHMM+DDd SMN> N=5. Table 4: <[HSM2001] HHMM+DDd NNN> N=44
=E=	Catalogue in electronic form as J/AJ/121/1840
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSM2009]
[HSM2009]	(Henry+Siana+Malkan+, 2009)
Write:	<<[HSM2009] CDFS-N-JD1>> <<[HSM2009] C5-zD1>> <<[HSM2009] C8-JD1>>
N:	4
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Search for galaxies at z=7-10 in GOODS, COSMOS, HST NICMOS SSA22 data.
Ref:	=2009ApJ...697.1128H
by	HENRY A.L. , SIANA B., MALKAN M.A., ASHBY M.L.N., BRIDGE C.R., CHARY R.-R., COLBERT J.W., GIAVALISCO M., TEPLITZ H.I., McCARTHY P.J.
	Astrophys. J., 697, 1128-1137 (2009)
	Expanding the search for galaxies at z ~ 7-10 with new NICMOS parallel fields.
o	Table 2: <[HSM2009] CDFS-N-JD1> N=2, <[HSM2009] C5-zD1>, <[HSM2009] C8-JD1>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSN2004]
[HSN2004]	(Hall+Snedden+Niederste-Ostholt+, 2004) (Not yet in Simbad)
Write:	<<[HSN2004] QSO J0952+0114 abs N.NNNN>> <<[HSN2004] Absorber A>>
N:	7
Object:	Absorber
Note:	Study of QSO J0952+0114 = SDSS J095253.83+011421.9: N=5 associated absorption systems (A to E) and N=2 intervening absorption systems.
Ref:	=2004AJ....128..534H
by	HALL P.B. , SNEDDEN S.A., NIEDERSTE-OSTHOLT M., EISENSTEIN D.J., STRAUSS M.A., YORK D.G., SCHNEIDER D.P.
	Astron. J., 128, 534-543 (2004)
	A quasar without broad Lyα emission.
o	Table 2: <[HSN2004] QSO J0952+0114 abs N.NNNN> N=7, = <[HSN2004] Absorber A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSN2010]
[HSN2010]	(Hester+Seibert+Neill+, 2010)
Write:	<<[HSN2010] aN>>
N:	9+3
Object:	Bright knot + Diffuse region (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	GALEX observations of IC 3418. Use of publicly available ESO 3.6m Hα observations.
in source:	IC 3418
Ref:	=2010ApJ...716L..14H
by	HESTER J.A. , SEIBERT M., NEILL J.D., WYDER T.K., GIL DE PAZ A., MADORE B.F., MARTIN D.C., SCHIMINOVICH D., RICH R.M.
	Astrophys. J., 716L, 14-18 (2010)
	IC 3418: star formation in a turbulent wake.
o	Fig. 1, Table 1: <[HSN2010] aN> (Nos k1-k9, d1-d3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSN2014]
[HSN2014]	(Hsu+Salvato+Nandra+, 2014)
Write:	<<[HSN2014] NNNNNN>>
N:	105176
Object:	G (SIMBAD class: Galaxy)
Note:	N=105176 sources in the CANDELS/GOODS-South field, the Chandra Deep Field South (CDFS) and the Extended Chandra Deep Field South (ECDFS).
in source:	NAME GOODS South Field
in source:	NAME CDFS
in source:	NAME ECDFS
Ref:	=2014ApJ...796...60H
by	HSU L.-T. , SALVATO M., NANDRA K., BRUSA M., BENDER R., BUCHNER J., DONLEY J.L., KOCEVSKI D.D., GUO Y., HATHI N.P., RANGEL C., WILLNER S.P., BRIGHTMAN M., GEORGAKAKIS A., BUDAVARI T., SZALAY A.S., ASHBY M.L.N., BARRO G., DAHLEN T., FABER S.M., FERGUSON H.C., GALAMETZ A., GRAZIAN A., GROGIN N.A., HUANG K.-H., KOEKEMOER A.M., LUCAS R.A., McGRATH E., MOBASHER B., PETH M., ROSARIO D.J., TRUMP J.R.
	Astrophys. J., 796, 60 (2014)
	CANDELS/GOODS-S, CDFS, and ECDFS : photometric redshifts for normal and X-Ray-detected galaxies.
o	Table 8: <[HSN2014] NNNNNN> (Nos 1-105176).
=E=	Catalogue in electronic form as <J/ApJ/796/60/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HSN2016]
[HSN2016]	(Hernan-Caballero+Spoon+Lebouteiller+, 2016)
Write:	<<[HSN2016] JDDD.dd+DD.dd>>
N:	?
Object:	G (SIMBAD class: Galaxy)
Note:	Identification of optical counterparts of the infrared sources detected in Spitzer IRS observations, as part of the Infrared Database of Extragalactic Observables from Spitzer (IDEOS).
Ref:	=2016MNRAS.455.1796H
by	HERNAN-CABALLERO A. , SPOON H.W.W., LEBOUTEILLER V., RUPKE D.S.N., BARRY D.P.
	Mon. Not. R. Astron. Soc., 455, 1796-1806 (2016)
	The infrared database of extragalactic observables from Spitzer - I. The redshift catalogue.
o	Table B1: <[HSN2016] JDDD.dd+DD.dd> N=?
=E=	Catalogue in electronic form as <J/MNRAS/455/1796/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSN2020]
[HSN2020]	(Huynh+Seymour+Norris+, 2020)
Write:	<<[HSN2020] NN>> <<[HSN2020] NNA>>
N:	55+22
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA 9.0GHz observations of N=55 radio galaxies (format NNN) and N=22 source components (format NNNA) in the extended Chandra Deep Field South, by the Australia Telescope Large Area Survey (ATLAS) team. See also ATCDFS9,, as well as [HHL2012], [HBH2015b].
in source:	NAME ECDFS
Ref:	=2020MNRAS.491.3395H
by	HUYNH M.T. , SEYMOUR N., NORRIS R.P., GALVIN T.
	Mon. Not. R. Astron. Soc., 491, 3395-3410 (2020)
	The ATLAS 9.0 GHz survey of the extended Chandra Deep Field South: the faint 9.0 GHz radio population.
o	Table 2, col(1): <[HSN2020] NN> N=55 among (Nos 1-70), <[HSN2020] NNA> N=22 among (Nos 14A-14D to 68A-68D). Table 2, col(2): <ATCDFS9 JHHMMSS.ss+DDMMSS.s> N=70.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HSNH
HSNH	(Handa+Sofue+Nakai+Hirabayashi+)
Write:	<<HSNH NNN>>
N:	144
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Identif. charts
Ref:	=1987PASJ...39..709H
by	HANDA T. , SOFUE Y., NAKAI N., HIRABAYASHI H., INOUE M.
	Publ. Astron. Soc. Jap., 39, 709-753 (1987)
	A radio continuum survey of the Galactic Plane at 10 GHz.
o	Table2: <HSNH NNN> (Nos 1-144)
Details on Acronym: HSO
HSO	(Herschel Space Observatory)= (HSOBMHERICC)
Write:	<<HSO PNHERICC JDDD.dddd+DD.dddd>> <<HSO SNHERICC JDDD.dddd+DD.dddd>> <<HSO BMHERICC JDDD.dddd+DD.dddd>>
N:	5062+10914+30910+27395+8424+42825
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	The HERschel Inventory of The Agents of Galaxy Evolution (HERITAGE) in the Magellanic Clouds project is a Herschel Space Observatory open time key program. The source name convention, for the point-source Catalogs, is an 11 character string, OOOIIPPPPEL, followed by source-specific position designation JRR.RRRRSDD.DDDD. HSO denotes the observatory, Herschel Space Observatory, HSO; II specifies the instrument (P for PACS, S for SPIRE, BM for band-matched) and the wavelength (2, 3, 1, 2, 3 for 100, 160, 250, 350, and 500 µm, respectively); PPPP is a four-character code for the HERITAGE project, HERI; E denotes the epoch (all sources are marked with C, combined-epoch detections), and L designates the list type, C for Catalog. RR.RRRR and DD.DDDD are the right ascension and declination, respectively, in degrees to four decimal places, and S is the sign of the declination.
Ref:	=2013AJ....146...62M
by	MEIXNER M. , PANUZZO P., ROMAN-DUVAL J., ENGELBRACHT C., BABLER B., SEALE J., HONY S., MONTIEL E., SAUVAGE M., GORDON K., MISSELT K., OKUMURA K., CHANIAL P., BECK T., BERNARD J.-P., BOLATTO A., BOT C., BOYER M.L., CARLSON L.R., CLAYTON G.C., CHEN C.-H.R., CORMIER D., FUKUI Y., GALAMETZ M., GALLIANO F., HORA J.L., HUGHES A., INDEBETOUW R., ISRAEL F.P., KAWAMURA A., KEMPER F., KIM S., KWON E., LEBOUTEILLER V., LI A., LONG K.S., MADDEN S.C., MATSUURA M., MULLER E., OLIVEIRA J.M., ONISHI T., OTSUKA M., PARADIS D., POGLITSCH A., REACH W.T., ROBITAILLE T.P., RUBIO M., SARGENT B., SEWILO M., SKIBBA R., SMITH L.J., SRINIVASAN S., TIELENS A.G.G.M., VAN LOON J.Th., WHITNEY B.
	Astron. J., 146, 62 (2013)
	The HERschel Inventory of The Agents of Galaxy Evolution in the Magellanic Clouds, a Herschel open time key program.
o	(Erratum) erratum vol. 149, art. 88 (2015)
o	lmcp100.dat, smcp100.dat: <HSO P2HERICC JDDD.dddd+DD.dddd> N=4164+898. lmcp160.dat, smcp160.dat: <HSO P3HERICC JDDD.dddd+DD.dddd> N=9324+1590. lmcp250.dat, smcp250.dat: <HSO S1HERICC JDDD.dddd+DD.dddd> N=25445+5465. lmcp350.dat, smcp350.dat: <HSO S2HERICC JDDD.dddd+DD.dddd> N=22082+5313. lmcp500.dat, smcp500.dat: <HSO S3HERICC JDDD.dddd+DD.dddd> N=7355+1069.
Ref:	=2014AJ....148..124S
by	SEALE J.P. , MEIXNER M., SEWILO M., BABLER B., ENGELBRACHT C.W., GORDON K., HONY S., MISSELT K., MONTIEL E., OKUMURA K., PANUZZO P., ROMAN-DUVAL J., SAUVAGE M., BOYER M.L., CHEN C.-H.R., INDEBETOUW R., MATSUURA M., OLIVEIRA J.M., SRINIVASAN S., VAN LOON J.Th., WHITNEY B., WOODS P.M.
	Astron. J., 148, 124 (2014)
	Herschel key program Heritage: a far-infrared source catalog for the Magellanic Clouds.
o	<HSO BMHERICC JDDD.dddd+DD.dddd> N=35322+7503.
=E=	Catalogue in electronic form as J/AJ/146/62
=E=	Catalogue in electronic form as <J/AJ/148/124/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HSO2006]
[HSO2006]	(Hennawi+Strauss+Oguri+, 2006)
Write:	<<[HSO2006] SDSS JHHMM+DDMMA>> <<[HSO2006] 2QZ JHHMM+DDMMA>>
N:	831+836
Object:	QSO (SIMBAD class: QSO = Quasar)
Note:	Sample of SDSS QSOs in pairs. See also [MRB2008].
Ref:	=2006AJ....131....1H
by	HENNAWI J.F. , STRAUSS M.A., OGURI M., INADA N., RICHARDS G.T., PINDOR B., SCHNEIDER D.P., BECKER R.H., GREGG M.D., HALL P.B., JOHNSTON D.E., FAN X., BURLES S., SCHLEGEL D.J., GUNN J.E., LUPTON R.H., BAHCALL N.A., BRUNNER R.J., BRINKMANN J.
	Astron. J., 131, 1-23 (2006)
	Binary quasars in the Sloan Digital Sky Survey: evidence for excess clustering on small scales.
o	Table 1 : Q1120+0195 incorrect for Q1120+019 (=UM 425, not UM 144 as mentioned in note 2)
o	Tables 2,3,4,8,9,10: <[HSO2006] SDSS JHHMM+DDMMA>, <[HSO2006] 2QZ JHHMM+DDMMA> N=890.
=E=	Catalogue in electronic form as J/AJ/131/1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSO2011]
[HSO2011]	(Hota+Sirotha+Ohyama+, 2011)
Write:	<<[HSO2011] WW middle lobe>> <<[HSO2011] WW outer relic lobe>>
N:	4
Object:	Lobe (SIMBAD class: Radio = Radio Source)
Note:	GMRT 325MHz observations of the radio galaxy Speca.
in source:	NAME Speca
Ref:	=2011MNRAS.417L..36H
by	HOTA A. , SIROTHIA S.K., OHYAMA Y., KONAR C., KIM S., REY S.-C., SAIKIA D.J., CROSTON J.H., MATSUSHITA S.
	Mon. Not. R. Astron. Soc., 417L, 36-40 (2011)
	Discovery of a spiral-host episodic radio galaxy.
o	<NAME Speca> N=1. Fig. 2: <[HSO2011] WW middle lobe> (Nos NW, SE), <[HSO2011] WW outer relic lobe> (Nos NW, SE).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HSOBMHERICC
HSOBMHERICC	(Herschel Space Observatory, Band-Matched HERITAGE Combined-epoch Catalog)
*****	Avoid the usage of HSOBMHERICC, prefer HSO
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HSP2005]
[HSP2005]	(Howell+Sullivan+Perrett+, 2005)
Write:	<<[HSP2005] JHHMMSS.sss+DDMMSS.ss>>
N:	64+61+38
Object:	G (SIMBAD class: Galaxy)
Note:	Gemini observations of SNs from the Supernova Legacy Survey SNLS. Each SN has an identified host galaxy identified.
Ref:	=2005ApJ...634.1190H
by	HOWELL D.A. , SULLIVAN M., PERRETT K., BRONDER T.J., HOOK I.M., ASTIER P., AUBOURG E., BALAM D., BASA S., CARLBERG R.G., FABBRO S., FOUCHEZ D., GUY J., LAFOUX H., NEILL J.D., PAIN R., PALANQUE-DELABROUILLE N., PRITCHET C.J., REGNAULT N., RICH J., TAILLET R., KNOP R., McMAHON R.G., PERLMUTTER S., WALTON N.A.
	Astrophys. J., 634, 1190-1201 (2005)
	Gemini Spectroscopy of Supernovae from the Supernova Legacy Survey: Improving High-Redshift Supernova Selection and Classification.
o	Tables 1, 2: <SNLS YYDNaa> N=64, <[HSP2005] JHHMMSS.sss+DDMMSS.ss> N=64.
Ref:	=2006A&A...447...31A
by	ASTIER P. , GUY J., REGNAULT N., PAIN R., AUBOURG E., BALAM D., BASA S., CARLBERG R.G., FABBRO S., FOUCHEZ D., HOOK I.M., HOWELL D.A., LAFOUX H., NEILL J.D., PALANQUE-DELABROUILLE N., PERRETT K., PRITCHET C.J., RICH J., SULLIVAN M., TAILLET R., ALDERING G., ANTILOGUS P., ARSENIJEVIC V., BALLAND C., BAUMONT S., BRONDER J., COURTOIS H., ELLIS R.S., FILIOL M., GONCALVES A.C., GOOBAR A., GUIDE D., HARDIN D., LUSSET V., LIDMAN C., McMAHON R., MOUCHET M., MOURAO A., PERLMUTTER S., RIPOCHE P., TAO C., WALTON N.
	Astron. Astrophys., 447, 31-48 (2006)
	The Supernova Legacy Survey: measurement of Ω_{M}, Ω_Λ and W from the first year data set.
o	reprint in the special issue (500/1) : 2009A&A...500..597A
o	Table 7: <SNLS YYDNaa> N=61 added. Table 7: <[HSP2005] JHHMMSS.sss+DDMMSS.ss> N=61 added.
Ref:	=2006AJ....132.1126N
by	NEILL J.D. , SULLIVAN M., BALAM D., PRITCHET C.J., HOWELL D.A., PERRETT K., ASTIER P., AUBOURG E., BASA S., CARLBERG R.G., CONLEY A., FABBRO S., FOUCHEZ D., GUY J., HOOK I., PAIN R., PALANQUE-DELABROUILLE N., REGNAULT N., RICH J., TAILLET R., ALDERING G., ANTILOGUS P., ARSENIJEVIC V., BALLAND C., BAUMONT S., BRONDER J., ELLIS R.S., FILIOL M., GONCALVES A.C., HARDIN D., KOWALSKI M., LIDMAN C., LUSSET V., MOUCHET M., MOURAO A., PERLMUTTER S., RIPOCHE P., SCHLEGEL D., TAO C.
	Astron. J., 132, 1126-1145 (2006)
	The type Ia supernova rate at z~0.5 from the Supernova Legacy Survey.
o	Table 2: <SNLS YYDNaa> N=38 added. Table 2: <[HSP2005] JHHMMSS.sss+DDMMSS.ss> N=38 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSP2006]
[HSP2006]	(Halkola+Seitz+Pannella, 2006)
Write:	<<[HSP2006] NN>> <<[HSP2006] Arc NN.a>>
N:	80+126
Object:	G in ClG + Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Use of archival HST WFPC2 and ACS data. N=80 galaxies in ACO 1689 and N=126 arcs (lensing images).
in source:	ACO 1689
Ref:	=2006MNRAS.372.1425H
by	HALKOLA A. , SEITZ S., PANNELLA M.
	Mon. Not. R. Astron. Soc., 372, 1425-1462 (2006)
	Parametric strong gravitational lensing analysis of Abell 1689.
o	Table B1: <[HSP2006] NN> (Nos 1-80). Table C1, Figs D: <[HSP2006] Arc NN.a> N=126.
=E=	Catalogue in electronic form as J/MNRAS/372/1425
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSP2011]
[HSP2011]	(Henderson+Stanek+Pejcha+, 2011)
Write:	<<[HSP2011] NNN>>
N:	121
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	MDM 1.3m McGraw-Hill telescope observations of N=121 variable stars in two fields centered on the Cygnus OB2 association.
in source:	NAME VI Cyg = Ass Cyg OB 2
Ref:	=2011ApJS..194...27H
by	HENDERSON C.B. , STANEK K.Z., PEJCHA O., PRIETO J.L.
	Astrophys. J., Suppl. Ser., 194, 27 (2011)
	An R- and I-band photometric variability survey of the Cygnus OB2 association.
o	Table 2: <[HSP2011] NNN> (Nos 1-121).
=E=	Catalogue in electronic form as <J/ApJS/194/27/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 3HSP
3HSP	(Third High Synchrotron Peaked blazar)
Write:	<<3HSP JHHMMSS.s+DDMMSS>>
N:	2013
Object:	Poss. Blazar (SIMBAD class: Blazar_Candidate = Blazar Candidate)
Stat:	is completely incorporated in Simbad
Note:	The third catalogue for High Synchrotron Peaked (HSP) blazars includes N=2013 sources. See also 1WHSP and 2WHSP. The W in the acronym has been removed in this edition of the catalogue as sources are no longer required to be detected in the WISE all sky survey.
Ref:	=2019A&A...632A..77C
by	CHANG Y.-L. , ARSIOLI B., GIOMMI P., PADOVANI P., BRANDT C.H.
	Astron. Astrophys., 632A, 77-77 (2019)
	The 3HSP catalogue of extreme and high-synchrotron peaked blazars.
o	Table 1: <3HSP JHHMMSS.s+DDMMSS> N=2013.
=E=	Catalogue in electronic form as <J/A+A/632/A77/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HSR2001]
[HSR2001]	(Holden+Stanford+Rosati+, 2001)
Write:	<<[HSR2001] Arc>> <<[HSR2001] Arc A>> <<[HSR2001] Group W>>
N:	1+2+2
Object:	Grav. Arc (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	In the HST image of RX J0848.8+4456, N=1 gravitational arc with 2 bright components A and B, and 2 faint components C and D found later. An other candidate image 'Arc T' is also found in the second ref. The cluster id divided in 2 sub-groups North and South.
Ref:	=2001AJ....122..629H
by	HOLDEN B.P. , STANFORD S.A., ROSATI P., SQUIRES G., TOZZI P., FOSBURY R.A.E., PAPOVICH C., EISENHARDT P., ELSTON R., SPINRAD H.
	Astron. J., 122, 629-636 (2001)
	RX J0848+4456: disentangling a moderate redshift cluster.
o	Fig.2: <[HSR2001] Group W> (Nos N, S). Fig.5: <[HSR2001] Arc> N=1, <[HSR2001] Arc A> (Nos A-B).
Ref:	=2003ApJ...596..797F
by	FOSBURY R.A.E. , VILLAR-MARTIN M., HUMPHREY A., LOMBARDI M., ROSATI P., STERN D., HOOK R.N., HOLDEN B.P., STANFORD S.A., SQUIRES G.K., RAUCH M., SARGENT W.L.W.
	Astrophys. J., 596, 797-809 (2003)
	Massive star formation in a gravitationally lensed H II galaxy at z = 3.357.
o	Fig.1: <[HSR2001] Arc A> (Nos C, D, T) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSS2004]
[HSS2004]
Write:	<<[HSS2004] NN>>
N:	20
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra and XMM-Newton observations of NGC 4214.
in source:	NGC 4214
Ref:	=2004MNRAS.348..406H
by	HARTWELL J.M. , STEVENS I.R., STRICKLAND D.K.
	Mon. Not. R. Astron. Soc., 348, 406-420 (2004)
	Chandra and XMM-Newton observations of NGC 4214: the hot interstellar medium and the luminosity function of dwarf starbursts.
o	Fig.1, Table 2: <[HSS2004] NN> (Nos 1-20).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSS2007]
[HSS2007]	(Hancock+Smith+Struck+, 2007)
Write:	<<[HSS2007] NN>>
N:	30
Object:	(FUV) (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	GALEX, SARA 0.9m telescope (Kitt Peak), and Spitzer observations of Arp 82 system.
in source:	APG 82A
in source:	APG 82B
Ref:	=2007AJ....133..676H
by	HANCOCK M. , SMITH B.J., STRUCK C., GIROUX M.L., APPLETON P.N., CHARMANDARIS V., REACH W.T.
	Astron. J., 133, 676-693 (2007)
	Large-scale star formation triggering in the low-mass Arp 82 system: a nearby example of galaxy downsizing based on UV/Optical/Mid-IR imaging.
o	Fig.2, Table 2: <[HSS2007] NN> (Nos 1-30).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSS2009]
[HSS2009]	(Hancock+Smith+Struck+, 2009)= ([HSS2009a]) (Not yet in Simbad)
Write:	<<[HSS2009] NN>>
N:	45
Object:	Clump (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	GALEX, SDSS and SARA 0.9m telescope observations of Arp 305.
in source:	APG 305
Ref:	=2009AJ....137.4643H
by	HANCOCK M. , SMITH B.J., STRUCK C., GIROUX M.L., HURLOCK S.
	Astron. J., 137, 4643-4654 (2009)
	Candidate tidal dwarf galaxies in Arp 305: lessons on dwarf detachment and globular cluster formation.
o	Tables 2-5: <[HSS2009] NN> (Nos 1-45).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSS2009a]
[HSS2009a]	(Hancock+Smith+Struck+, 2009) (Not yet in Simbad)
*****	Avoid the usage of [HSS2009a], prefer [HSS2009]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSS2009b]
[HSS2009b]	(Hilton+Stanford+Stott+, 2009)
Write:	<<[HSS2009b] NNNN>>
N:	64
Object:	G (SIMBAD class: Galaxy)
Note:	HST ACS and Subaru MOIRCS observations of XMMXCS J2215.9-1738.
in source:	XMMXCS J2215.0-1738
Ref:	=2009ApJ...697..436H
by	HILTON M. , STANFORD S.A., STOTT J.P., COLLINS C.A., HOYLE B., DAVIDSON M., HOSMER M., KAY S.T., LIDDLE A.R., LLOYD-DAVIES E., MANN R.G., MEHRTENS N., MILLER C.J., NICHOL R.C., ROMER A.K., SABIRLI K., SAHLEN M., VIANA P.T.P., WEST M.J., BARBARY K., DAWSON K.S., MEYERS J., PERLMUTTER S., RUBIN D., SUZUKI N.
	Astrophys. J., 697, 436-451 (2009)
	The XMM cluster survey: galaxy morphologies and the color-magnitude relation in XMMXCS J2215.9-1738 at z = 1.46.
o	Table 1: <[HSS2009b] NNNN> N=64 among (Nos 8-1243).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSS2021]
[HSS2021]	(Hughes+Sand+Seth+, 2021)= (H21)
Write:	<<[HSS2021] NNNNNN>>
N:	474916
Object:	Poss. GlCl + G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=474916 sources (globular cluster candidates, background galaxies, foreground stars) in the field of NGC 5128, based on data from the Panoramic Imaging Survey of Centaurus and Sculptor (PISCeS). See also [HSS2023].
in source:	Cen A = NGC 5128
Ref:	=2021ApJ...914...16H
by	HUGHES A.K. , SAND D.J., SETH A., STRADER J., VOGGEL K., DUMONT A., CRNOJEVIC D., CALDWELL N., FORBES D.A., SIMON J.D., GUHATHAKURTA P., TOLOBA E.
	Astrophys. J., 914, 16-16 (2021)
	NGC 5128 globular cluster candidates out to 150 kpc: a comprehensive catalog from Gaia and ground-based data.
o	Table 2: <[HSS2021] NNNNNN> (Nos 1-474916).
=E=	Catalogue in electronic form as <J/ApJ/914/16/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [HSS2023]
[HSS2023]	(Hughes+Sand+Seth+, 2023)= (H22)
Write:	<<[HSS2023] NNN>>
N:	97
Object:	GlCl + G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Magellan M2FS and AATAAOmega observations of N=97 sources (globular cluster, background galaxies, foreground stars) in the field of NGC 5128. See also [HSS2021].
in source:	Cen A = NGC 5128
Ref:	=2023ApJ...947...34H
by	HUGHES A.K. , SAND D.J., SETH A., STRADER J., LIDMAN C., VOGGEL K., DUMONT A., CRNOJEVIC D., MATEO M., CALDWELL N., FORBES D.A., PEARSON S., GUHATHAKURTA P., TOLOBA E.
	Astrophys. J., 947, 34 (2023)
	New Velocity Measurements of NGC 5128 Globular Clusters Out to 130 kpc: Outer Halo Kinematics, Substructure, and Dynamics.
o	Tables 3-5: <[HSS2023] NNN> N=97 among (Nos 3-446).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [HSS84]
[HSS84]	(Hauser+Silverberg+Stier+, 1984)
Write:	<<[HSS84] NN>>
N:	80
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=80 submillimetric sources
Ref:	=1984ApJ...285...74H
by	HAUSER M.G. , SILVERBERG R.F., STIER M.T., KELSALL T., GEZARI D.Y., DWEK E., WALSER D., MATHER J.C., CHEUNG L.H.
	Astrophys. J., 285, 74-88 (1984)
	Submillimeter wavelength survey of the galactic plane from l=-5 to l=+62 : structure and energetics of the inner disk.
o	Table 3: <[HSS84] NN> (Nos 1-80)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSS98]
[HSS98]	(Hester+Stapelfeldt+Scowen, 1998)
Write:	<<[HSS98] HH 1 Arch N>> <<[HSS98] HH 1 Shoulder N>> <<[HSS98] HH 1 Faint N>>
N:	3+2+2
Object:	Knot (SIMBAD class: HerbigHaroObj = Herbig-Haro Object)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC 2 observations. See also [EMB94]
in source:	HH 1
Ref:	=1998AJ....116..372H
by	HESTER J.J. , STAPELFELDT K.R., SCOWEN P.A.
	Astron. J., 116, 372-395 (1998)
	Hubble space telescope wide field planetary camera 2 observations of HH 1-2.
o	The other knots in HH NNN objects have a format 'HH NNNA' or 'HH NNNAN'. The 2 diffraction features 'D.S'' in Fig.6, without numbering, are not in SIMBAD.
o	Fig.3: <[EMB94] HH 1 ANJ> (Nos G3J, G4J, F1J, F2J) added. Figs 6, 7: <[HSS98] HH 1 Arch N> (Nos 1-3), <[HSS98] HH 1 Shoulder N> (Nos 1-2), <[HSS98] HH 1 Faint N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSS99]
[HSS99]	(Hines+Schmidt+Smith, 1999)
Write:	<<[HSS99] Star WW>>
N:	3
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	3 stars in the field of the QSO 'NAME APM 08279+5255'
Ref:	=1999ApJ...514L..91H
by	HINES D.C. , SCHMIDT G.D., SMITH P.S.
	Astrophys. J., 514, 91-94 (1999)
	The polarized spectrum of APM 08279+5255.
o	Table 1: <[HSS99] Star WW> (Nos W, SW, E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HST
HST	(Hubble Space Telescope)
*****	Avoid the usage of HST, prefer [BSD98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HST
HST	(Hubble Space Telescope)
*****	Avoid the usage of HST, prefer [CBS98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HST
HST	(Hubble Space Telescope)
*****	Avoid the usage of HST, prefer [DWG95]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HST
HST	(Hubble Space Telescope)
*****	Avoid the usage of HST, prefer [FSB98]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HST
HST	(Hubble Space Telescope)
*****	Avoid the usage of HST, prefer [GRN94]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HST
HST	(Hubble Space Telescope)
*****	Avoid the usage of HST, prefer [LS2001]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HST
HST	(Hubble Space Telescope)
*****	Avoid the usage of HST, prefer [MMN2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HST
HST	(Hubble Space Telescope)
*****	Avoid the usage of HST, prefer [OW94]
Origin	of the Acronym: L (1998ApJ...499..758J)
Details on Acronym: HST
HST	(Hubble Space Telescope)
*****	Avoid the usage of HST, prefer [OWH93]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HST
HST	(Hubble Space Telescope)
*****	Avoid the usage of HST, prefer [PBZ99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HST
HST	(Hubble Space Telescope)
*****	Avoid the usage of HST, prefer [RGO99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HST
HST	(Hubble Space Telescope)
*****	Avoid the usage of HST, prefer [ROG95]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HST
HST	(Hubble Space Telescope)
*****	Avoid the usage of HST, prefer [RSC2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HST
HST	(Hubble Space Telescope)
*****	Avoid the usage of HST, prefer [YBG2005]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HST PC
HST PC	(Hubble Space Telescope)
*****	Avoid the usage of HST PC, prefer PSH
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HST-uvnova
HST-uvnova	(HST, UV)
*****	Avoid the usage of HST-uvnova, prefer [MSF2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HST77]
[HST77]	(Hintzen+Scott+Tarenghi, 1977)
Write:	<<[HST77] NN>>
N:	14
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	N=14 galaxies in ACO 401. Map Fig.1.
in source:	ACO 401
Ref:	=1977ApJ...212....8H
by	HINTZEN P. , SCOTT J.S., TARENGHI M.
	Astrophys. J., 212, 8-12 (1977)
	The velocity dispersion of Abell 401.
o	Table 1: <[HST77] NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HST94]
[HST94]	(Hughes+Stetson+Turner+, 1994)
Write:	<<[HST94] V30 NN>> <<[HST94] MA NN>>
N:	49+16
Object:	* (SIMBAD class: Star)
Note:	Table 4: format 'V30 NN', N=49 secondary standards in the field 'V30'. format 'MA NN', N=16 secondary standards in the 'Major Axis' field. See also: [FHM94], [KIF96], [FFH96], [SHM96], [GPF97], [RMM97], [FBK98], [HHH98], [PSF98], [TFS98], [GHS99], [KIS99], [SHF99], [GFF99], [MHS99], [SFK99], [PKB99], [GSF2000], [MHS2000]
in source:	M 81 = NGC 3031
Ref:	=1994ApJ...428..143H
by	HUGHES S.M.G. , STETSON P.B., TURNER A., KENNICUTT R.C., HILL R., LEE M.G., FREEDMAN W.L., MOULD J.R., MADORE B.F., FERRARESE L., FORD H.C., GRAHAM J.A., HOESSEL J.G., ILLINGWORTH G.D.
	Astrophys. J., 428, 143-156 (1994)
	The Hubble Space Telescope extragalactic distance scale key project. II. Photometry of WFC images of M 81.
o	Table 4: <[HST94] V30 NN> (Nos 1-49), <[HST94] MA NN> (Nos 1-16)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HSTGC
HSTGC	(Hubble Space Telescope, Guide Catalog)
*****	Avoid the usage of HSTGC, prefer GSC
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HSTNGC602
HSTNGC602	(SMC star cluster NGC602 (HST/ACS Optical Sources))
Write:	<<HSTNGC602 JHHMMSS.sss+DDMMSS.ss>>
N:	about 4500
Object:	stars, forming stars (SIMBAD class: Star)
Note:	This is a detailed study of star-forming cluster NGC 602 in the wing of the SMC. This is an optical source list from Hubble Space Telescope imaging with resolution of 0".02/pix Deep infrared observations were also performed on the region by Fazio upon the commissioning of the Spitzer Space Telescope. This accompanying acronym request is for designations SSTNGC602 JHHMMSS.ss+DDMMSS.s (note: fewer decimal places quoted in SST than HST). See also SSTNGC602. Matches between the SST and HST sources will be noted, also matches to Hutchings 1991, Goulermis 2007, and Schmalzl 2008. Massey 2002 is outside our field of view; Westerlund 1963 includes no coordinate list. Carlson 2007 and Cignoni 2009 use this photometry list.
Auth.:	Lynn Redding Carlson Johns Hopkins University / Space Telescope Science Institute
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [HSV99]
[HSV99]	(Huovelin+Schultz+Vilhu+, 1999) (Not yet in Simbad)
Write:	<<[HSV99] NN>>
N:	10
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	New BeppoSAX X-ray sources in the EXS 1737.9-2952 region.
Ref:	=1999A&A...349L..21H
by	HUOVELIN J. , SCHULTZ J., VILHU O., HANNIKAINEN D., MUHLI P., DUROUCHOUX P.
	Astron. Astrophys., 349, 21-24 (1999)
	BeppoSAX observations of the EXS 1737.9-2952 region. I. Discovery of new X-ray sources.
o	Table 1: <[HSV99] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HSVMT
HSVMT	(Heithausen+Stacy+de Vries+Mebold+Thaddeus)= ([HSD93a])
Write:	<<HSVMT NN>>
N:	29
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Ref:	=1993A&A...268..265H
by	HEITHAUSEN A. , STACY J.G., DE VRIES H.W., MEBOLD U., THADDEUS P.
	Astron. Astrophys., 268, 265-275 (1993)
	A composite large-scale CO survey at high galactic latitudes in the second quadrant.
o	<HSVMT NN> (Nos 1-29)
Origin	of the Acronym: L (1996ApJS..106..447M)
Details on Acronym: [HSW2005]
[HSW2005]	(Houck+Soifer+Weedman+, 2005)= (Houck) = (SST24)
Write:	<<[HSW2005] NN>> <<[HSW2005] SST24 JHHMMSS.ss+DDMMSS.s>> <<[HSW2005] JHHMMSS.s+DDMMSS>> (not recognised by Simbad, but found in literature)
N:	17+1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Observations of a field within the NOAO Deep Wide-Field Survey (NDWFS) region in Bootes with the Spitzer Space Telescope. See also [WLH2006], [WSH2006], [HWL2007].
Ref:	=2005ApJ...622L.105H
by	HOUCK J.R. , SOIFER B.T., WEEDMAN D., HIGDON S.J.U., HIGDON J.L., HERTER T., BROWN M.J.I., DEY A., JANNUZI B.T., LE FLOC'H E., RIEKE M., ARMUS L., CHARMANDARIS V., BRANDL B.R., TEPLITZ H.I.
	Astrophys. J., 622, 105-108 (2005)
	Spectroscopic redshifts to z > 2 for optically obscured sources discovered with the Spitzer Space Telescope.
o	Table 1: <[HSW2005] NN> (Nos 1-17) = <[HSW2005] SST24 JHHMMSS.ss+DDMMSS.s> N=17.
Ref:	=2006ApJ...641..133D
by	DESAI V. , ARMUS L., SOIFER B.T., WEEDMAN D.W., HIGDON S., BIAN C., BORYS C., SPOON H.W.W., CHARMANDARIS V., BRAND K., BROWN M.J.I., DEY A., HIGDON J., HOUCK J., JANNUZI B.T., LE FLOC'H E., ASHBY M.L.N., SMITH H.A.
	Astrophys. J., 641, 133-139 (2006)
	IRS spectra of two ultraluminous infrared galaxies at z = 1.3.
o	<[HSW2005] SST24 JHHMMSS.ss+DDMMSS.s> N=1 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSW2010]
[HSW2010]	(Husemann+Sanchez+Wisotzki+, 2010)
Write:	<<[HSW2010] SN>>
N:	2
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=2 faint shells on a HST F606W broad-band image of the host galaxy of HE 1029-1401.
Ref:	=2010A&A...519A.115H
by	HUSEMANN B. , SANCHEZ S.F., WISOTZKI L., JAHNKE K., KUPKO D., NUGROHO D., SCHRAMM M.
	Astron. Astrophys., 519A, 115-115 (2010)
	Mapping the ionised gas around the luminous QSO He 1029-1401: evidence for minor merger events?
o	Fig. 1: <[HSW2010] SN> (Nos S1-S2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSW2018]
[HSW2018]	(Higuchi+Sakai+Watanabe+, 2018)
Write:	<<[HSW2018] NGC 1333-NN>> <<[HSW2018] L1448-N>> <<[HSW2018] IC 348-N>> <<[HSW2018] Barnard 5>> <<[HSW2018] B1-N>> <<[HSW2018] L1455-N>> <<[HSW2018] L1527>>
N:	36+1
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	Nobeyama 45m and IRAM 30m telescope C2H, c-C3H2 and CH3OH line observations of N=36 YSOs in the Perseus molecular cloud complex.
in source:	NAME Perseus Molecular Cloud
Ref:	=2018ApJS..236...52H
by	HIGUCHI A.E. , SAKAI N., WATANABE Y., LOPEZ-SEPULCRE A., YOSHIDA K., OYA Y., IMAI M., ZHANG Y., CECCARELLI C., LEFLOCH B., CODELLA C., BACHILLER R., HIROTA T., SAKAI T., YAMAMOTO S.
	Astrophys. J., Suppl. Ser., 236, 52-52 (2018)
	Chemical survey toward young stellar objects in the Perseus molecular cloud complex.
o	Table 1: <[HSW2018] NGC 1333-NN> (Nos 1-17), <[HSW2018] L1448-N> (Nos 1-5), <[HSW2018] IC 348-N> (Nos 1-4), <[HSW2018] Barnard 5> N=1, <[HSW2018] B1-N> (Nos 1-5), <[HSW2018] L1455-N> (Nos 1-4).
Ref:	=2018ApJ...869...51I
by	IMAI M. , SAKAI N., LOPEZ-SEPULCRE A., HIGUCHI A.E., ZHANG Y., OYA Y., WATANABE Y., SAKAI T., CECCARELLI C., LEFLOCH B., YAMAMOTO S.
	Astrophys. J., 869, 51-51 (2018)
	Deuterium fractionation survey toward protostellar sources in the Perseus molecular cloud: HNC case.
o	Table 1: <[HSW2018] L1527> N=1 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HSW99]
[HSW99]	(Huard+Sandell+Weintraub, 1999)= (SMM)
Write:	<<[HSW99] CB NNN SMM N>> <<[HSW99] B NNN SMM N>> <<[HSW99] L NNN SMM Na>>
N:	17+2
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SCUBA observations on JCMT. N=17 Submillimeter sources in 8 large globules.
in source:	[CB88] 3
in source:	[CB88] 34
in source:	[CB88] 68
in source:	[CB88] 146
in source:	[CB88] 230
in source:	[CB88] 232
in source:	Barnard 335
in source:	LDN 810
Ref:	=1999ApJ...526..833H
by	HUARD T.L. , SANDELL G., WEINTRAUB D.A.
	Astrophys. J., 526, 833-844 (1999)
	Submillimeter maps of Bok globule cores: evidence for multiple epoch star formation.
o	Table 2: <[HSW99] CB 68 SMM N> (No. 1), <[HSW99] CB 146 SMM N> (Nos 1-2), <[HSW99] B 335 SMM N> (No. 1), <[HSW99] CB 230 SMM N> (No. 1), <[HSW99] CB 232 SMM N> (Nos 1-2).
Ref:	=2000A&A...362..635H
by	HUARD T.L. , WEINTRAUB D.A., SANDELL G.
	Astron. Astrophys., 362, 635-645 (2000)
	Submillimeter maps of small young clusters in three large globules.
o	Table 1: <[HSW99] CB 3 SMM N> (No. 1), <[HSW99] CB 34 SMM N> (Nos 1-5), <[HSW99] L 810 SMM N> (Nos 1-2).
Ref:	=2006A&A...457..891C
by	CODELLA C. , BRAND J., MASSI F., WOUTERLOOT J.G.A., DAVIS G.R.
	Astron. Astrophys., 457, 891-897 (2006)
	Inside the large globule CB205: YSOs feeding multiple outflows.
o	Table 1: <[HSW99] L 810 SMM Na> (Nos 3, 4, 1a, 1b) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HT
HT	(Heydari-Malayeri+Testor)
*****	Avoid the usage of HT, prefer [HT83]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HT2008]
[HT2008]	(Houghton+Thatte, 2008)
Write:	<<[HT2008] NN>>
N:	17
Object:	Young Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	VLT ISAAC near-IR spectroscopy and archival HST WFPC2 images to study the central region of M 83.
in source:	M 83 = NGC 5236
Ref:	=2008MNRAS.385.1110H
by	HOUGHTON R.C.W. , THATTE N.
	Mon. Not. R. Astron. Soc., 385, 1110-1128 (2008)
	The central region of M83.
o	Fig.7, Table 4: <[HT2008] NN> (Nos 1-17).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HT76]
[HT76]	(Herbst+Turner, 1976)= ([NCG85])
Write:	<<[HT76] NN>>
N:	12
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-6) in ref. 1976PASP...88..308H, (Nos 7-12) in ref. 1985A&A...153..253N, already described as red nebulous obj, in fig. 1, 1st ref.
in source:	LDN 810
Ref:	=1976PASP...88..308H
by	HERBST W. , TURNER D.G.
	Publ. Astron. Soc. Pac., 88, 308-311 (1976)
	Lynds 810 - An interesting globule in northern Vulpecula.
o	Table 1: <[HT76] N> (Nos 1-6)
Ref:	=1985A&A...153..253N
by	NECKEL T. , CHINI R., GUSTEN R., WINK J.E.
	Astron. Astrophys., 153, 253-259 (1985)
	Star formation in the large globule L 810.
o	Text and Fig. 1: <[HT76] NN> (Nos 7-12) added. Fig 1a: <[NCG85] IR N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HT82]
[HT82]	(Heydari-Malayeri+Testor, 1982)
Write:	<<[HT82] N159AN>> <<[HT82] N159A ggg>> <<[HT82] N>>
N:	2+4+5
Object:	Region + * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Fig.1, 2: N159A (LHA 120-N 159A) has 2 components 'N159A1' and 'N159A2', and 4 brightness peaks: (alf, bet, gam, del). Fig.2, text: (Nos 1-4) are stars in the field of LHA 120-N 159, (No. 5) is a peculiar object name 'Blob'. See also [HT86], [HVL90].
in source:	Magellanic Clouds:LMC:LHA 120-N 159A = LHA 120-N 159A
Ref:	=1982A&A...111L..11H
by	HEYDARI-MALAYERI M. , TESTOR G.
	Astron. Astrophys., 111, 11-14 (1982)
	Excitation and extinction in the LMC HII region N159A and discovery of a highly excited 'Blob' in its vicinity.
o	DD 13 = [DD75] LMC X-1 13.
o	Figs 1, 2: <[HT82] N159AN> (Nos A1-A2), <[HT82] N159A aaa> (Nos alf, bet, gam, del), <[HT82] N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HT83]
[HT83]	(Heydari-Malayeri+Testor)= (HT)
Write:	<<[HT83] N>> <<[HT83] alf>> <<[HT83] HD 32228 aN>>
N:	4+1+19
Object:	(Opt) + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	(Nos 1-4), N=4 small discrete objects. (No. alf), N=1 group of stars. HD 32228 is a multiple system, resolved in components (Nos a-l, b1-b2, g1-g3, h1-h2).
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1983A&A...118..116H
by	HEYDARI-MALAYERI M. , TESTOR G.
	Astron. Astrophys., 118, 116-122 (1983)
	Optical observations of the LMC HII region N 11.
o	Fig 1a: <[HT83] N> (Nos 1-4), <[HT83] alf> N=1. Fig.6: <[HT83] HD 32228 a> (Nos a-l).
Ref:	=1999AJ....118.1684W
by	WALBORN N.R. , DRISSEN L., PARKER J.W., SAHA A., MacKENTY J.W., WHITE R.L.
	Astron. J., 118, 1684-1699 (1999)
	HST/FOS spatially resolved spectral classification of compact OB groups in the Large Magellanic Cloud.
o	LH 10-3209 is [L72] LH 10-3209 = PGMW 3209 in SIMBAD.
o	Table 1: <[WDP99] Brey 73 NN> N=23 among (Nos 1-28). Table 2: <[WDP99] NGC 2044W NN> N=37 among (Nos 1-45). Table 3: <[WDP99] LH 10-3209 NN> (Nos 14-19) = <[WDP99] LH 10-3209 A> (Nos A-F). Table 4: <[WDP99] HD 32228 NN> N=71 among (Nos 1-98). Fig.5, Table 2: <[HGM93] NNAa> (Nos 5Aa, 5Ab, 5D, 5E) added. Fig.12, Table 4: <[HT83] HD 32228 aN> (Nos b1-b2, g1-g3, h1-h2) added.
=E=	Catalogue in electronic form as <J/AJ/118/1684/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HT86]
[HT86]	(Heydari-Malayeri+Testor, 1986)
Write:	<<[HT86] N160AN>> <<[HT86] NNN>>
N:	3+215
Object:	Region + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Fig.1a: N160A (LHA 120-N 160A) has 3 components 'N160A1' to 'N160A3'. N160A1 and A2 are 2 Blobs in LHA 120-N 160. Table 2, Fig.1f: (Nos 1-215), stars in the field of LHA 120-N 160. See also [HT82], [HVL90].
in source:	Magellanic Clouds:LMC:LHA 120-N 160A = LHA 120-N 160A
Ref:	=1986A&A...162..180H
by	HEYDARI-MALAYERI M. , TESTOR G.
	Astron. Astrophys., 162, 180-198 (1986)
	Detection and study of two HII blobs in the LMC giant HII region N 160 and investigation of their nebular and stellar environment.
o	Table 2, Fig.1f: <[HT86] NNN> (Nos 11-215). Fig.1Aa: <[HT86] N160AN> (Nos A1-A3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HT95]
[HT95]	(Hunter+Thronson, 1995)
Write:	<<[HT95] Star NNN>> <<[HT95] HII NN>>
N:	398+15
Object:	* + HII (SIMBAD class: Star)
Note:	see also [CSG2002].
in source:	Zw I 18 = Mrk 116
Ref:	=1995ApJ...452..238H
by	HUNTER D.A. , THRONSON H.A.Jr
	Astrophys. J., 452, 238-252 (1995)
	The massive stars of I Zw 18 as seen in Hubble Space Telescope images.
o	Table 2: <[HT95] Star NNN> (Nos 1-398). Table 5: <[HT95] HII NN> (Nos 1-15)
=E=	Catalogue in electronic form as J/ApJ/452/238
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTA2017]
[HTA2017]	(Hacar+Tafalla+Alves, 2017)
Write:	<<[HTA2017] NN>>
N:	50
Object:	NH3 Core (SIMBAD class: denseCore = Dense Core)
Note:	Effelsberg 100m and IRAM 30m telescopes NH3 and N2H+ lines observations in the NGC 1333 region in Perseus. Use of archival Herschel and Planck data.
in source:	NGC 1333
Ref:	=2017A&A...606A.123H
by	HACAR A. , TAFALLA M., ALVES J.
	Astron. Astrophys., 606A, 123-123 (2017)
	Fibers in the NGC 1333 proto-cluster.
o	Table 2: <[HTA2017] NN> (Nos 1-50).
=E=	Catalogue in electronic form as <J/A+A/606/A123/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTB2006]
[HTB2006]	(Hill+Thompson+Burton+, 2006)
Write:	<<[HTB2006] GLLL.ll+BB.bb>> <<[HTB2006] GLLL.lll+BB.bbb>>
N:	212
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	SCUBA observations: 212 submillimeter cores are identified, including the 106 millimeter sources known from the SIMBA survey (see [HBM2005]).
Ref:	=2006MNRAS.368.1223H
by	HILL T. , THOMPSON M.A., BURTON M.G., WALSH A.J., MINIER V., CUNNINGHAM M.R., PIERCE-PRICE D.
	Mon. Not. R. Astron. Soc., 368, 1223-1268 (2006)
	Millimetre continuum observations of southern massive star formation regions - II. SCUBA observations of cold cores and the dust grain emissivity index (β).
o	Table 3: <[HTB2006] GLLL.ll+BB.bb>, <[HTB2006] GLLL.lll+BB.bbb>, N=212. Table 4: <[HBM2005] GLLL.lll+BB.bbb> N=2 added.
=E=	Catalogue in electronic form as J/MNRAS/368/1223
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTB2020]
[HTB2020]	(Hermosa Munoz+Taibi+Battaglia+, 2020)
Write:	<<[HTB2020] aquNcNstarNN>>
N:	53
Object:	RGB* (SIMBAD class: RGB* = Red Giant Branch star)
Note:	VLT FORS2/MXU observations of N=53 RGB stars in the Aquarius dwarf galaxy.
in source:	DDO 210 = NAME Aquarius Dwarf Galaxy
Ref:	=2020A&A...634A..10H
by	HERMOSA MUNOZ L. , TAIBI S., BATTAGLIA G., IORIO G., REJKUBA M., LEAMAN R., COLE A.A., IRWIN M., JABLONKA P., KACHAROV N., McCONNACHIE A., STARKENBURG E., TOLSTOY E.
	Astron. Astrophys., 634A, 10-10 (2020)
	Kinematic and metallicity properties of the Aquarius dwarf galaxy from FORS2 MXU spectroscopy.
o	Table A.2: <[HTB2020] acquNcNstarNN> N=53.
=E=	Catalogue in electronic form as <J/A+A/634/A10/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTC2014]
[HTC2014]	(Holwerda+Trenti+Clarkson+, 2014)
Write:	<<[HTC2014] BoRG HHMM+DDMM.NNNN.N>>
N:	30+1+274
Object:	BD* (SIMBAD class: BrownD* = Brown Dwarf)
Note:	Identification of N=30+1+374 L, T and M dwarfs in the Brightest of Reionizing Galaxies survey (BoRG). Use of HST WFC3 imaging from the CANDELS and ERS surveys in the GOODS-South Field.
Ref:	=2014ApJ...788...77H
by	HOLWERDA B.W. , TRENTI M., CLARKSON W., SAHU K., BRADLEY L., STIAVELLI M., PIRZKAL N., DE MARCHI G., ANDERSEN M., BOUWENS R., RYAN R.
	Astrophys. J., 788, 77 (2014)
	Milky Way red dwarfs in the BoRG survey: galactic scale-height and the distribution of dwarf stars in WFC3 imaging.
o	(Erratum) erratum vol. 825, art. 82 (2016)
o	Tables 14-16: <[HTC2014] BoRG HHMM+DDMM.NNNN.N> N=30+1+274.
=E=	Catalogue in electronic form as <J/ApJ/788/77/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTC94]
[HTC94]	(Huang+Thuan+Chevalier+, 1994)
Write:	<<[HTC94] NN>> <<[HTC94] SS.s+SS.s>>
N:	50
Object:	SNR + Poss. SNR (SIMBAD class: SNRemnant_Candidate = SuperNova Remnant Candidate)
Stat:	is completely incorporated in Simbad
Note:	The format 'SS.s+SS.s' is to be avoided, offset relative to RA = 09h51m, Dec = +69deg54' (1950). 'SS.s' are the seconds of RA (.s is rounded), and '+SS.s' are the rounded seconds of Dec.
in source:	M 82 = NGC 3034
Ref:	=1994ApJ...424..114H
by	HUANG Z.P. , THUAN T.X., CHEVALIER R.A., CONDON J.J., YIN Q.F.
	Astrophys. J., 424, 114-125 (1994)
	Compact radio sources in the starburst galaxy M 82 and the σ-D relation for supernova remnants.
o	RA: 9h51' Dec: +69° 54'
o	Table 1: <[HTC94] NN> or <[HTC94] SS.s+SS.s> N=50
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HtDe
HtDe	(Hartl+Dengel+)
*****	Avoid the usage of HtDe, prefer HDW
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HTF2008]
[HTF2008]	(Huxor+Tanvir+Ferguson+, 2008)
Write:	<<[HTF2008] HNN>> <<[HTF2008] HECNN>>
N:	27+13
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Note:	INT WFC and CFHT Megacam observations of M 31.
in source:	M 31 = NGC 224
Ref:	=2008MNRAS.385.1989H
by	HUXOR A.P. , TANVIR N.R., FERGUSON A.M.N., IRWIN M.J., IBATA R., BRIDGES T., LEWIS G.F.
	Mon. Not. R. Astron. Soc., 385, 1989-1997 (2008)
	Globular clusters in the outer halo of M31: the survey.
o	Figs 1, 2, Table 1: <[HTF2008] HNN> (Nos H1-H27). Fig. 3, Table 2: <[HTF2008] HECNN> (Nos HEC1-HEC13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTF94]
[HTF94]	(Hunter+Taylor+Felli+, 1994)
Write:	<<[HTF94] W75N N>>
N:	5
Object:	H2O Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
in source:	W 75
Ref:	=1994A&A...284..215H
by	HUNTER T.R. , TAYLOR G.B., FELLI M., TOFANI G.
	Astron. Astrophys., 284, 215-226 (1994)
	Water masers embedded in ultracompact HII regions : the W 75N cloud core.
o	Table 1: <[HTF94] W75N N> (Nos 1-5). Table 2, Fig.1: <[HRB81] W75N(Ba)> (Nos Ba-Bd).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTH2012]
[HTH2012]	(Hatchell+Terebey+Huard+, 2012)
Write:	<<[HTH2012] OphN Na>>
N:	7
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	Spitzer IRAC and MIPS observations of N=7 molecular clouds in the Ophiuchus North (Oph N).
Ref:	=2012ApJ...754..104H
by	HATCHELL J. , TEREBEY S., HUARD T., MAMAJEK E.E., ALLEN L., BOURKE T.L., DUNHAM M.M., GUTERMUTH R., HARVEY P.M., JORGENSEN J.K., MERIN B., NORIEGA-CRESPO A., PETERSON D.E.
	Astrophys. J., 754, 104 (2012)
	The Spitzer survey of interstellar clouds in the Gould Belt. V. Ophiuchus North observed with IRAC and MIPS.
o	Objects [HTH2012] OphN Na are not in SIMBAD.
o	Tables 1-2: <[HTH2012] OphN Na> (Nos 1-2, 3a, 3b, 4-6). Tables 5,7: <SSTgbs JHHMMSSs+DDMMSS> N=15.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTI2003]
[HTI2003]	(Hunt+Thuan+Izotov, 2003) (Not yet in Simbad)
Write:	<<[HTI2003] WWN>> <<[HTI2003] W(WW)>> <<[HTI2003] Int>>
N:	10
Object:	Region (SIMBAD class: Region = Region defined in the Sky)
Note:	JHK images of Zw I 18, and analyze in conjunction with archival HST WFPC2 images. See [DKF89].
in source:	Zw I 18 = Mrk 116
Ref:	=2003ApJ...588..281H
by	HUNT L.K. , THUAN T.X., IZOTOV Y.I.
	Astrophys. J., 588, 281-298 (2003)
	New light on the populations in I Zw 18: deep near-infrared imaging.
o	Table 1, Fig.3: <[HTI2003] WWN> (Nos NW, SE, NW1-NW2, SE1-SE2), <[HTI2003] W(WW)> (Nos C, C(NW), C(SE)), <[HTI2003] Int> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTI2015]
[HTI2015]	(Hatsukade+Tamura+Iono+, 2015)
Write:	<<[HTI2015] NN>>
N:	14
Object:	CO Cloud (SIMBAD class: MolCld = Molecular Cloud)
Note:	ALMA CO(5-4) emission line observations of N=14 molecular clouds in the gravitationally lensed submillimeter galaxy H-ATLAS J090311.6+003906 (SDP.81).
in source:	SDP 81
Ref:	=2015PASJ...67...93H
by	HATSUKADE B. , TAMURA Y., IONO D., MATSUDA Y., HAYASHI M., OGURI M.
	PASJ, 67, 93 (2015)
	High-resolution ALMA observations of SDP.81. II. Molecular clump properties of a lensed submillimeter galaxy at z = 3.042.
o	Table 1: <[HTI2015] NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTK2008]
[HTK2008]	(Hashimoto+Tamura+Kandori+, 2008)
Write:	<<[HTK2008] IRN R-N>>
N:	18
Object:	IR RfNeb (SIMBAD class: RefNeb = Reflection Nebula)
Stat:	is completely incorporated in Simbad
Note:	SAAO IRSF 1.4m telescope SIRIUS and SIRPOL observations. NIR linear polarization images of NGC 6334 region. N=18 infrared reflexion nebulae are found.
in source:	NGC 6334
Ref:	=2008ApJ...677L..39H
by	HASHIMOTO J. , TAMURA M., KANDORI R., KUSAKABE N., NAKAJIMA Y., KURITA M., NAGATA T., NAGAYAMA T., HOUGH J., CHRYSOSTOMOU A.
	Astrophys. J., 677L, 39-42 (2008)
	Wide-field infrared imaging polarimetry of the NGC 6334 region: a nest of infrared reflection nebulae.
o	Table 1: <[HTK2008] IRN R-N> (Nos I-1 to I-5, II-1 to II-2, III-1 to III-2, IV-1 to IV-6, V-1 to V-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTK2013]
[HTK2013]	(Hacar+Tafalla+Kauffmann+, 2013)
Write:	<<[HTK2013] NN>>
N:	19
Object:	Dense Core (SIMBAD class: denseCore = Dense Core)
Note:	FCRAO 14m telescope N2H+(1-0) observations of N=19 dense cores in L1495/B213 complex in Taurus.
in source:	LDN 1495
in source:	Barnard 213
Ref:	=2013A&A...554A..55H
by	HACAR A. , TAFALLA M., KAUFFMANN J., KOVACS A.
	Astron. Astrophys., 554A, 55-55 (2013)
	Cores, filaments, and bundles: hierarchical core formation in the L1495/B213 Taurus region.
o	Table 2: <[HTK2013] NN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTK2018]
[HTK2018]	(Hayashi+Tadaki+Kodama+, 2018)
Write:	<<[HTK2018] ALMA.B7.NN>>
N:	9
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ALMA band 7 dust continuum observations of N=9 galaxies in the XMMXCS J2215.9-1738 galaxy cluster at z=1.46. See also [SSS2017] and [HKK2017].
in source:	XMMXCS J2215.9-1738
Ref:	=2018ApJ...856..118H
by	HAYASHI M. , TADAKI K.-I., KODAMA T., KOHNO K., YAMAGUCHI Y., HATSUKADE B., KOYAMA Y., SHIMAKAWA R., TAMURA Y., SUZUKI T.L.
	Astrophys. J., 856, 118-118 (2018)
	Molecular gas reservoirs in cluster galaxies at z = 1.46.
o	Table 1, Fig. 2: <[HTK2018] ALMA.B7.NN> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTL92]
[HTL92]	(Hewitt+Turner+Lawrence+, 1992)
Write:	<<[HTL92] MG J0414+0534 system>> <<[HTL92] A>> <<[HTL92] AN>> <<[HTL92] Aa>> <<[HTL92] ANa>> <<[HTL92] Star N>> <<[HTL92] Star A>> <<[HTL92] gN>>
N:	1+4+2+6+3
Object:	(Rad)+ Grav. lens system + Grav. lensed image + * + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=3 radio-knots in MITG J0414+0534, (Nos A-C), No. A divided into A1, A2. In 2000, these knots are divided into 16 VLBI components, 'Aa' and 'ANa', with 'a' standing for p, q, ,r, s components. N=6 standard stars in the field of MITG J0414+0534, 'Star 1 to Star 6' (1st and 2nd ref.). N=1 fortuitous 'Star M' (fig. 3, 1st ref.). N=1 new object found in 2nd ref., 'X' N=1 Lensing Galaxy 'G', found in 2nd ref. N=3 galaxies 'g1 to g3', found in 3rd ref.
in source:	MITG J0414+0534
Ref:	=1992AJ....104..968H
by	HEWITT J.N. , TURNER E.L., LAWRENCE C.R., SCHNEIDER D.P., BRODY J.P.
	Astron. J., 104, 968-979 (1992)
	A gravitational lens candidate with an unusually red optical counterpart.
o	<[HTL92] MG J0414+0534 system> N=1. Table 2, fig.1: <[HTL92] A> (Nos A-C), <[HTL92] AN> (Nos A1-A2). Table 4, fig.3: <[HTL92] Star N> (Nos 1-3), <[HTL92] Star M>
Ref:	=1993AJ....105....1S
by	SCHECHTER P.L. , MOORE C.B.
	Astron. J., 105, 1-6 (1993)
	The lensing galaxy in MG 0414+0534.
o	MG 0414+0534 = MITG J0414+0534. The lensing galaxy is [HTL92] G in 1997AJ.113.340F
o	Table 4: <[HTL92] Star N> (Nos 1-6), (Nos 4-6) are new. Fig.1: <[HTL92] G>, <[HTL92] X> are new
Ref:	=1994A&A...281..388A
by	ANGONIN-WILLAIME M.-C. , VANDERRIEST C., HAMMER F., MAGAIN P.
	Astron. Astrophys., 281, 388-394 (1994)
	Further observational evidence that MG J0414+0534 is a gravitational mirage.
o	(Erratum) erratum vol. 292 p.722 (1994)
o	Table 2: <[HTL92] gN> (Nos g1-g3)
Ref:	=2000ApJ...535..671T
by	TROTTER C.S. , WINN J.N., HEWITT J.N.
	Astrophys. J., 535, 671-691 (2000)
	A multipole-Taylor expansion for the potential of the gravitational lens MG J0414+0534.
o	Table 1, Fig.2: <[HTL92] ANa> (Nos A1p-A1s, Nos A2p-A2s), <[HTL92] Aa> (Nos Bp-Bs, Cp-Cs).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTM83]
[HTM83]	(Harris+Townes+Matsakis+, 1983)
Write:	<<[HTM83] Cloudet A>>
N:	2
Object:	Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	Description of two small cloud fragments (or clumps) in OMC 1. They are called 'Cloudet A' and 'Cloudet B' in 1999A&AS..134..241P.
Ref:	=1983ApJ...265L..63H
by	HARRIS A. , TOWNES C.H., MATSAKIS D.N., PALMER P.
	Astrophys. J., 265, 63-66 (1983)
	Small rotating clouds of stellar mass in Orion Molecular Cloud 1.
o	<[HTM83] Cloudet A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTM99]
[HTM99]	(Hara+Tachihara+Mizuno+, 1999)
Write:	<<[HTM99] NN>> <<[HTM99] GLLL.l+BB.b>>
N:	36
Object:	MCld (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	Observations with the NANTEN telescope. N=36 C18O cores in Lupus cloud complex.
in source:	NAME Lupus Cloud
Ref:	=1999PASJ...51..895H
by	HARA A. , TACHIHARA K., MIZUNO A., ONISHI T., KAWAMURA A., OBAYASHI A., FUKUI Y.
	Publ. Astron. Soc. Jap., 51, 895-910 (1999)
	A study of dense cloud cores and star formation in Lupus: CO J = 1-0 observations with NANTEN.
o	Table 1: <[HTM99] NN> (Nos 1-36) = <[HTM99] GLLL.l+BB.b> N=36. Table 1, last column: <Lupus N> (Nos 6-9) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTN2002]
[HTN2002]	(Hjorth+Thomsen+Nielsen+, 2002)
Write:	<<[HTN2002] A>>
N:	9
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Objects in the field of GRB 980613. Objects (Nos A-E) were already published in astro-ph/0008029 in 2000, object A is the host galaxy of the GRB.
Ref:	=2002ApJ...576..113H
by	HJORTH J. , THOMSEN B., NIELSEN S.R., ANDERSEN M.I., HOLLAND S.T., FYNBO J.U., PEDERSEN H., JAUNSEN A.O., HALPERN J.P., FESEN R., GOROSABEL J., CASTRO-TIRADO A., McMAHON R.G., HOENIG M.D., BJORNSSON G., AMATI L., TANVIR N.R., NATARAJAN P.
	Astrophys. J., 576, 113-119 (2002)
	The afterglow and complex environment of the optically dim burst GRB 980613.
o	(Nos A-E) were already designated in Djorgovski+, Astro-ph 0008029, not published.
o	Table 2, Figs: <[HTN2002] A> (Nos A-K, D and E missing).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTN2003]
[HTN2003]	(Habart+Testi+Natta+, 2003)
Write:	<<[HTN2003] MWC 297 N>> <<[HTN2003] V921 Sco N>> <<[HTN2003] LSS 3027B N>> <<[HTN2003] VY Mon N>> <<[HTN2003] HD 97048 N>>
N:	11
Object:	(Mid IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	ESO La Silla 3.6m telescope TIMMI2 observations. Mid-IR observations of 5 fields.
Ref:	=2003A&A...400..575H
by	HABART E. , TESTI L., NATTA A., VANZI L.
	Astron. Astrophys., 400, 575-583 (2003)
	Mid-IR observations of small stellar clusters surrounding Herbig AeBe stars.
o	T.2: LSS 3027B = [ST89] LSS 3027 B in SIMBAD
o	Table 2: <[HTN2003] MWC 297 N> (Nos 1-2), <[HTN2003] V921 Sco N> (Nos 1-4), <[HTN2003] LSS 3027B N> (No. 1), <[HTN2003] VY Mon N> (Nos 1-2), <[HTN2003] HD 97048 N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTP2005]
[HTP2005]	(Hily-Blant+Teyssier+Philipp+, 2005)
Write:	<<[HTP2005] Peak N>>
N:	4
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	IRAM 30m HERA C18O(2-1) observations of the Horsehead Nebula.
in source:	Horsehead Nebula = Barn 33
Ref:	=2005A&A...440..909H
by	HILY-BLANT P. , TEYSSIER D., PHILIPP S., GUESTEN R.
	Astron. Astrophys., 440, 909-919 (2005)
	Velocity field and star formation in the Horsehead nebula.
o	Paragr. 3.1: <[HTP2005] Peak N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HTR
HTR	(HATNet TRansit candidate) (Not yet in Simbad)
*****	Avoid the usage of HTR, prefer [BFV2016]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HTR
HTR	(Hyland+Thomas+Robinson)
Write:	<<HTR NN>>
N:	24
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-8, 10-11, 13-24) are identical to MHR numbering, but 1981ApJ...250..116M is not considered as a continuation of 1978AJ.....83...20H, 'MH' being used in the literature as the usual acronym.
in source:	Magellanic Clouds:LMC:30 Dor Nebula = 30 Dor Nebula
Ref:	=1978AJ.....83...20H
by	HYLAND A.R. , THOMAS J.A., ROBINSON G.
	Astron. J., 83, 20-25 (1978)
	Infrared studies of 30 Doradus. I. The 2-µ sources of the inner region.
o	Table 1: <HTR NN> (Nos 1-24).
Origin	of the Acronym: L (1981ApJ...250..116M)
Details on Acronym: HTR
HTR	(HATNet TRansit candidate)
*****	Avoid the usage of HTR, prefer [LBT2009]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HTS2007]
[HTS2007]	(Hashimoto+Tamura+Suto+, 2007)
Write:	<<[HTS2007] WN-A>> <<[HTS2007] WN-AN>>
N:	4+5
Object:	Nebula + Knot (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Subaru telescope IR images of NGC 6334V = MFSW V.
in source:	NGC 6334:MFSW V = MFSW V
Ref:	=2007PASJ...59..221H
by	HASHIMOTO J. , TAMURA M., SUTO H., ABE L., ISHII M., KUDO T., MAYAMA S.
	PASJ, 59, 221-225 (2007)
	Subarcsecond near-infrared images of massive star formation region NGC 6334V.*
o	Fig.1, text: <[HTS2007] WN-A> (Nos EN-A, EN-B, WN-A, WN-B). Table 1: <[HTS2007] WN-AN> (Nos EN-A1 to EN-A3, WN-A1 to WN-A2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTS88]
[HTS88]	(Hewitt+Turner+Schneider+, 1988)
Write:	<<[HTS88] J1131+0456 AN>>
N:	4+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	(Nos A-D, A1-A2) radio components of MITG J1131+0456. D is the central object. See also (IR) components [A92].
in source:	MITG J1131+0456
Ref:	=1988Natur.333..537H
by	HEWITT J.N. , TURNER E.L., SCHNEIDER D.P., BURKE B.F., LANGSTON G.I., LAWRENCE C.R.
	Nature, 333, 537-540 (1988)
	Unusual radio source MG 1131+0456 : a possible Einstein ring.
o	Figs 1, 2: <[HTS88] J1131+0456 AN> (Nos A-C, A1-A2).
Ref:	=1993AJ....106.1719C
by	CHEN G.H. , HEWITT J.N.
	Astron. J., 106, 1719-1728 (1993)
	Multifrequency radio images of the Einstein ring gravitational lens.
o	Table 2: <[HTS88] J1131+0456 A> (No. D) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTT2020]
[HTT2020]	(Hibon+Tang+Thomas, 2020)
Write:	<<[HTT2020] LAB1>>
N:	1
Object:	Poss. Lyman Alpha Nebula (SIMBAD class: EmObj = Emission Object)
Note:	N=1 Lymanα nebula (or blob, LAB) candidate in the COSMOS field. Use of CFHT Legacy Deep survey data.
in source:	NAME COSMOS Field
Ref:	=2020A&A...641A..32H
by	HIBON P. , TANG F., THOMAS R.
	Astron. Astrophys., 641A, 32-32 (2020)
	A Lyα nebula at z ~ 3.3.
o	Figs 1-2, Table 1: <[HTT2020] LAB1> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTT95]
[HTT95]	(Hunter+Testi+Taylor+, 1995)= (IRS)
Write:	<<[HTT95] Maser NNW>> <<[HTT95] IR NN>> <<[HTT95] IRS N>> <<[HTT95] Knot AN>>
N:	13+30+2+26
Object:	Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Objects in AFGL 5142 region: N=13 H2O maser components, format 'Maser NNW', components of '[TGA92] AFGL 5142 H2O Maser'. See [TGA92]. N=30 * with excess IR, format 'IR NN'. N=2 IR Sources, format 'IRS N'. N=26+1 knots (Nos A-Z, Y1).
Ref:	=1995A&A...302..249H
by	HUNTER T.R. , TESTI L., TAYLOR G.B., TOFANI G., FELLI M., PHILLIPS T.G.
	Astron. Astrophys., 302, 249-263 (1995)
	A multiwavelength picture of the AFGL 5142 star-forming region.
o	Table 1: <[HTT95] Maser N> (Nos 1-5). Table 2: <[HTT95] IR NN> (Nos 1-30), <[HTT95] IRS N> (Nos 1-2). Table 3: <[HTT95] Knot A> (Nos A-F)
Ref:	=1999AJ....118..477H
by	HUNTER T.R. , TESTI L., ZHANG Q., SRIDHARAN T.K.
	Astron. J., 118, 477-487 (1999)
	Molecular jets and H_{2}O masers in the AFGL 5142 hot core.
o	Table 1: <[HTT95] Maser NNW> (Nos 3E, 4E, 6-11) added.
Ref:	=2005ApJ...629..288C
by	CHEN Y. , YAO Y., YANG J., ZENG Q., SATO S.
	Astrophys. J., 629, 288-298 (2005)
	Near-infrared imaging of the star formation region AFGL 5142.
o	Table 2: <[CYY2005] NIRS NNN> (Nos 1-164). Table 3: <[HTT95] Knot AN> (Nos G-Z, Y1) added.
=E=	Catalogue in electronic form as J/ApJ/629/288
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HtTr
HtTr	(Hartl+Tritton)
*****	Avoid the usage of HtTr, prefer HaTr
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HTU2003]
[HTU2003]	(Ho+Terashima+Ulvestad, 2003)
Write:	<<[HTU2003] X-N>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra X-ray sources the center of M 32. See also CXOM32
in source:	M 32 = NGC 221
Ref:	=2003ApJ...589..783H
by	HO L.C. , TERASHIMA Y., ULVESTAD J.S.
	Astrophys. J., 589, 783-789 (2003)
	Detection of the ``Active'' nucleus of M32.
o	Table 1: <[HTU2003] X-N> (Nos X-1 to X-3) = <CXOM32 JHHMMSS.s+DDMMSS> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTU2012]
[HTU2012]	(Hindson+Thompson+Urquhart+, 2012)
Write:	<<[HTU2012] NN>>
N:	71
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA observations at 5.5 and 8.8GHz of N=71 compact radio sources in the G305 star-forming complex.
in source:	GAL 305.2+00.2
Ref:	=2012MNRAS.421.3418H
by	HINDSON L. , THOMPSON M.A., URQUHART J.S., FAIMALI A., CLARK J.S., DAVIES B.
	Mon. Not. R. Astron. Soc., 421, 3418-3430 (2012)
	The G305 star-forming complex: a wide-area radio survey of ultracompact H II regions.
o	Table 2: <[HTU2012] NN> (Nos 0-70).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTU2013]
[HTU2013]	(Hindson+Thompson+Urquhart+, 2013)
Write:	<<[HTU2013] NNN>> <<[HTU2013] GLLL.lll+BB.bbb>>
N:	156+21
Object:	MCld + (Rad) (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	ATNF Mopra 22m radio telescope 12CO, 13CO and C18O and ATCA 5.5 and 8.8GHz continuum observations of the G305 star-forming complex: N=156 molecular clumps, and N=21 extended radio continuum sources.
in source:	NAME G305 complex = GAL 305.4+00.1
Ref:	=2013MNRAS.435.2003H
by	HINDSON L. , THOMPSON M.A., URQUHART J.S., FAIMALI A., JOHNSTON-HOLLITT M., CLARK J.S., DAVIES B.
	Mon. Not. R. Astron. Soc., 435, 2003-2022 (2013)
	The G305 star-forming complex: radio continuum and molecular line observations.
o	In Table 6, G305.270±0.007 is a probable misprint for G305.270-0.007. Calibrator PMN J1352-63 is not in Simbad.
o	Tables 3-4: <[HTU2013] NNN> (Nos 1-156). Table 6: <[HTU2013] GLLL.ll+BB.bbb> N=21.
=E=	Catalogue in electronic form as <J/MNRAS/435/2003/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTU2020]
[HTU2020]	(Higurashi+Tsuji+Uchiyama, 2020) (Not yet in Simbad)
Write:	<<[HTU2020] HSNN>>
N:	65
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS observations of N=65 point-like X-ray sources (hotspots) in the field of the RX J1713.7-3946 (SNR G347.3-00.5).
in source:	SNR G347.3-00.5
Ref:	=2020ApJ...899..102H
by	HIGURASHI R. , TSUJI N., UCHIYAMA Y.
	Astrophys. J., 899, 102-102 (2020)
	X-ray hotspots in the northwest shell of the supernova remnant RX J1713.7-3946.
o	Table 2: <[HTU2020] HSNN> (Nos HS01-HS65).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTV2001]
[HTV2001]	(Hulleman+Tennant+Van Kerkwijk+, 2001)
Write:	<<[HTV2001] A>> <<[HTV2001] A'>> <<[HTV2001] NN>> <<[HTV2001] XN>>
N:	12+2+13+7
Object:	? + (X) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Keck LRIS and Chandra ACIS observations. Fig.1, Table 1: Selected objects in the field of 1E 2259+58.6. Table 2: N=7 Chandra X-ray sources in the same field.
Ref:	=2001ApJ...563L..49H
by	HULLEMAN F. , TENNANT A.F., VAN KERKWIJK M.H., KULKARNI S.R., KOUVELIOTOU C., PATEL S.K.
	Astrophys. J., 563, 49-52 (2001)
	A possible faint near-infrared counterpart to the anomalous X-ray pulsar 1E 2259+586.
o	Table 1, Fig.1: <[HTV2001] A> N=12 among (Nos A-N), <[HTV2001] A'> (Nos B', L'), <[HTV2001] NN> (Nos 1-13). Table 2: <[HTV2001] XN> (Nos X1-X7).
=E=	Catalogue in electronic form as J/ApJ/563/L49
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HTV82]
[HTV82]	(Hoag+Thomas+Vaucher, 1982)
Write:	<<[HTV82] HHMMSS.s+DDMMSS>>
N:	23+20
Object:	Em* (SIMBAD class: EmObj = Emission Object)
Note:	Table 1: N=23 em-line obj. in Coma field. Table 2: N=20 em-line obj. in Coma blank field
Ref:	=1982ApJ...263...23H
by	HOAG A.H. , THOMAS N.G., VAUCHER B.G.
	Astrophys. J., 263, 23-31 (1982)
	Coma Quasars.
o	Tables 2, 3: <[HTV82] HHMMSS.s+DDMMSS> N=23+20
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Hu
Hu	(Hu)
Write:	<<Hu NNa>>
N:	36+14
Object:	HI Shell (SIMBAD class: HIshell = Interstellar Shell)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-36): 36 HI shells. format NNa: N=14 subshells clustering around larger shells
Ref:	=1981ApJ...248..119H
by	HU E.M.
	Astrophys. J., 248, 119-127 (1981)
	High latitude H I shells in the galaxy. I.
o	<Hu NNa> (Nos 1-36), N=50
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Hu
Hu	(Humason)
Write:	<<PN Hu 1-N>> <<PN Hu 2-N>>
N:	2+1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	PN Nomenclature. List 1: 1-N, N=2. List 2: 2-N, N=1, Hu 2-1 = PN G051.4+09.6 = PK 051+09 1
Ref:	=1921PASP...33..175H
by	HUMASON M.L.
	Publ. Astron. Soc. Pac., 33, 175-175 (1921)
	Two new planetary nebulae.
o	<PN Hu 1-N> (Nos 1-1, 1-2).
Ref:	=1922PASP...34..296H
by	HUMASON M.L.
	Publ. Astron. Soc. Pac., 34, 296-297 (1922)
	A new planetary nebula.
o	<PN Hu 2-N> (No. 2-1).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HU2001]
[HU2001]	(Ho+Ulvestad, 2001)
Write:	<<[HU2001] JHHMMSS.sss+DDMMSS.ss>> <<[HU2001] JHHMMSS.ss+DDMMSS.s>> <<[HU2001] JHHMMSS.s+DDMMSS>>
N:	116+134
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA Palomar observations of Seyfert galaxies. Table 3: N=116 sources in the center of the galaxies. Table 4: N=134 background sources in the fields of the galaxies.
Ref:	=2001ApJS..133...77H
by	HO L.C. , ULVESTAD J.S.
	Astrophys. J., Suppl. Ser., 133, 77-118 (2001)
	Radio continuum survey of an optically selected sample of nearby Seyfert galaxies.
o	Components measured in Table 3 not in SIMBAD.
o	Table 3: <[HU2001] JHHMMSS.sss+DDMMSS.ss>, <[HU2001] JHHMMSS.ss+DDMMSS.s>, N=116. Table 4: <[HU2001] JHHMMSS.s+DDMMSS> N=134.
=E=	Catalogue in electronic form as J/ApJS/133/77
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Hub
Hub	(Hubble)
*****	Avoid the usage of Hub, prefer Hb
Details on Acronym: Hubb
Hubb	(Hubble)
====>	Equivalent to: Hubble
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: Hubble
Hubble	(Hubble)
*****	Avoid the usage of Hubble, prefer BASW
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Hubble
Hubble	(Hubble)
*****	Avoid the usage of Hubble, prefer [H25]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Hubble
Hubble	(Hubble)
*****	Avoid the usage of Hubble, prefer [H29]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Hubble
Hubble	(Hubble)
*****	Avoid the usage of Hubble, prefer [H32]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Hubble
Hubble	(Hubble)= Hubb
Write:	<<Hubble I NN>> <<Hubble II NN>>
N:	33+29
Object:	Neb. Obj. (SIMBAD class: ISM = Interstellar Medium Object)
Note:	Table I: format 'I NN', N=33 diffuse neb. with continuous spectra (ex. IC 348, Pleiades..). Table II: format 'II NN', N=29 diffuse neb. with em. spectra (ex. NGC 1499, NGC 6611..).
Ref:	=1922ApJ....56..162H
by	HUBBLE E.P.
	Astrophys. J., 56, 162-199 (1922)
	A general study of diffuse galactic nebulae.
o	Table I: <Hubble I NN> (Nos 1-33). Table II: <Hubble II NN> (Nos 1-29)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Hubble
Hubble	(Hubble)
*****	Avoid the usage of Hubble, prefer Hb
Details on Acronym: Hubble
Hubble	(Hubble)
*****	Avoid the usage of Hubble, prefer VHK
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HuBi
HuBi	(Hu+Bibo)
Write:	<<PN HuBi N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Ref:	=1990A&A...234..435H
by	HU J.Y. , BIBO E.A.
	Astron. Astrophys., 234, 435-438 (1990)
	Discovery of a new cool WR star in a low excitation planetary nebula.
o	<PN HuBi 1>
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HUDF
HUDF	(Hubble Ultra Deep Field)
*****	Avoid the usage of HUDF, prefer [OCS2009]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HUDF
HUDF	(Hubble Ultra Deep Field)
*****	Avoid the usage of HUDF, prefer UDF
Origin	of the Acronym: L (2007AJ....134..169X)
Details on Acronym: HuDo
HuDo	(Hu+Dong)
Write:	<<PN HuDo N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	PN HuDo 1 = PN G060.4+01.5. 1991, Science Bull. of Academia Sinica
Auth.:	HU J.Y.+
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HUGS
HUGS	(HST UV Globular cluster Survey)
Write:	<<HUGS NGC NNNN RNNNNNNN>>
N:	?
Object:	* (SIMBAD class: Star)
Note:	Astrophotometric catalogues of 56 globular clusters and one open cluster, as part of the final data release of the project ‘HST UV Globular cluster Survey’ (HUGS). For more information, visit: http://groups.dfa.unipd.it/ESPG/treasury.php https://archive.stsci.edu/prepds/hugs/
Ref:	=2018MNRAS.481.3382N
by	NARDIELLO D. , LIBRALATO M., PIOTTO G., ANDERSON J., BELLINI A., APARICIO A., BEDIN L.R., CASSISI S., GRANATA V., KING I.R., LUCERTINI F., MARINO A.F., MILONE A.P., ORTOLANI S., PLATAIS I., VAN DER MAREL R.P.
	Mon. Not. R. Astron. Soc., 481, 3382-3393 (2018)
	The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters - XVII. Public Catalogue Release.
o	<HUGS NGC NNNN RNNNNNNN> N=?
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HuLo
HuLo	(Hua+Louise)
Write:	<<HuLo N>>
N:	1
Object:	Poss. PN (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
Note:	The nebulosity near NGC 6751 is called 'HuLo 1' in Acker+ 1992ESOPN...1....1A catalogue of PN.
Ref:	=1990A&A...235..403H
by	HUA C.T. , LOUISE R.
	Astron. Astrophys., 235, 403-406 (1990)
	The emission line nebulosity near the planetary nebula NGC 6751.
o	<HuLo 1> N=1
Origin	of the Acronym: L (1992ESOPN...1....1A)
Details on Acronym: HUNN
HUNN	(H.U. Norgaard-Nielsen+)
*****	Avoid the usage of HUNN, prefer [LNJ2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HuR
HuR	(Hu+Ridgway)
*****	Avoid the usage of HuR, prefer [HR94]
Origin	of the Acronym: L (2003ApJ...588...99B)
Details on Acronym: [HUW91]
[HUW91]	(Herbertz+Ungerechts+Winnewisser, 1991) (Not yet in Simbad)
Write:	<<[HUW91] A>> <<[HUW91] AN>>
N:	12+34
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Note:	Table 1: N=12 fragments (Nos A-L) in NGC 1499, each fragment containing several clumps 'AN'
in source:	NGC 1499
Ref:	=1991A&A...249..483H
by	HERBERTZ R. , UNGERECHTS H., WINNEWISSER G.
	Astron. Astrophys., 249, 483-492 (1991)
	CO observations of fragmentation in dark clouds north of the California nebula NGC 1499.
o	Table 1: <[HUW91] A> (Nos A-L), <[HUW91] AN> N=34
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Hux
Hux	(Huxor+)
*****	Avoid the usage of Hux, prefer M31WFS
Origin	of the Acronym: L (2006AJ....132.1571V)
Details on Acronym: HV
HV	(Hodge+, Variable ) (Not yet in Simbad)*
Write:	<<HV NNNNN>>
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Hodge + Wright Atlas of the LMC (1967) and the SMC (1977). Table 12 in the Hodge + Wright Atlas of the LMC (1967). Table 13 in the Hodge + Wright Atlas of the SMC (1977).
in source:	Magellanic Clouds:LMC = LMC
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1967SAOP.4699....1H
by	HODGE P.W. , WRIGHT F.W.
	SAO Publications, 4699, 1-None (1967)
	The Large Magellanic Cloud.
o	Atlas of the LMC.
Details on Acronym: HV
HV	(Wright+Hodge, 1974) (Not yet in Simbad)
*****	Avoid the usage of HV, prefer [WH74]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HV
HV	(Harvard univ., Variable *)
Write:	<<*SV HV** NNNNN>>
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Systematic designation. V* nomenclature.
Details on Acronym: [HV2002]
[HV2002]	(Hoyle+Vogeley+, 2002) (Not yet in Simbad)
Write:	<<[HV2002] PSCz NN>> <<[HV2002] UZC NN>>
N:	25+19
Object:	Void (SIMBAD class: Void = Underdense Region of the Universe)
Note:	Search for PSCz and UZC voids. See also [EP97b], [EPD97], [PB2002].
Ref:	=2002ApJ...566..641H
by	HOYLE F. , VOGELEY M.S.
	Astrophys. J., 566, 641-651 (2002)
	Voids in the Point Source Catalogue survey and the Updated Zwicky Catalog.
o	Voids are not numbered in the tables, but some of them are numbered in the text.
o	Table 1: <[HV2002] PSCz NN> (Nos 1-25). Table 2<[HV2002] UZC NN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HV86]
[HV86]	(Hummel+van der Hulst, 1986)= (HvdH)
Write:	<<[HV86] NNA>>
N:	15+4+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
in source:	NAME the Antennae
Ref:	=1986A&A...155..151H
by	HUMMEL E. , VAN DER HULST J.M.
	Astron. Astrophys., 155, 151-160 (1986)
	NGC 4038/4039: interacting spiral galaxies with enhanced extended radio emission.
o	Table 2: <[HV86] NN> (Nos 1-13)
Ref:	=2000AJ....120..670N
by	NEFF S.G. , ULVESTAD J.S.
	Astron. J., 120, 670-696 (2000)
	VLA observations of the nearby merger NGC 4038/4039: H II regions and supernova remnants in the "Antennae".
o	Calibrator J1159-2148 is PKS J1159-2148. SN 1921 = SN 1921A. Fig.11: (FUV) regions = [NHH96] UV NN. Fig.12: (X) = [FSM97] XNN.
o	Table 5: <[NU2000] NNA NN> N=109. Table 6: <[HV86] NNA> (Nos 1A, 2A, 4A-4B, 14-15) added.
Ref:	=2007A&A...466..467S
by	SCHULZ A. , HENKEL C., MUDERS D., MAO R.Q., ROELLIG M., MAUERSBERGER R.
	Astron. Astrophys., 466, 467-479 (2007)
	The interstellar medium of the Antennae galaxies.
o	Fig.2: <[WSM2000] SGMC N> (No. 0) added. Fig.2: <[HV86] NNA> (No. 13N) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HV93]
[HV93]	(Hawkins+Veron, 1993)
Write:	<<[HV93] a-NN>>
N:	48+79
Object:	QSO (SIMBAD class: QSO = Quasar)
Note:	Table 2(a): format 'a-NN', N=48, FOCAP sample. Table 2(b): format 'b-NN', N=79, bright sample.
Ref:	=1993MNRAS.260..202H
by	HAWKINS M.R.S. , VERON P.
	Mon. Not. R. Astron. Soc., 260, 202-208 (1993)
	The quasar luminosity function from a variability-selected sample.
o	Table 2(a): <[HV93] a-NN> N=48. Table 2(b): <[HV93] b-NN> N=79
=E=	Catalogue in electronic form as J/MNRAS/260/202
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HV95]
[HV95]	(Hawkins+Veron, 1995)
Write:	<<[HV95] a-NNN>> <<[HV95] b-NNN>> <<[HV95] c-NN>>
N:	111+117+86
Object:	QSO (SIMBAD class: QSO = Quasar)
Note:	extends [HV93], a - fibre field sample, b - bright sample, c - high redshift
Ref:	=1995MNRAS.275.1102H
by	HAWKINS M.R.S. , VERON P.
	Mon. Not. R. Astron. Soc., 275, 1102-1116 (1995)
	The evolution of the quasar luminosity function.
o	<[HV95] a-NNN> (Nos 1-111), <[HV95] b-NNN> (Nos 1-117), <[HV95] c-NN> (Nos 1-86)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HV96]
[HV96]	(Hibbart+Van Gorkom, 1996)
Write:	<<[HV96] Arp 295 GN>> <<[HV96] Arp 295 a>> <<[HV96] NGC 4676 a>> <<[HV96] NGC 4676 W>> <<[HV96] NGC 7252 WW>>
N:	9+2+2+1+1
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
in source:	APG 295
in source:	NGC 4676
in source:	NGC 7252
Ref:	=1996AJ....111..655H
by	HIBBARD J.E. , VAN GORKOM J.H.
	Astron. J., 111, 655-695 (1996)
	H I, H II, and R-band observations of a galactic merger sequence.
o	Table 7: <[HV96] Arp 295 GN> (Nos G1-G9), <[HV96] Arp 295 a> (Nos a-b), <[HV96] NGC 4676 a> (Nos a-b), <[HV96] NGC 4676 W> No. S, <[HV96] NGC 7252 WW> No. NE
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HVABG
HVABG	(Higgs+Vallee+Albinson+Batrla+Goss)
Write:	<<HVABG NNA>>
N:	42
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Table 4: (Nos 1-42) with 7 double sources (A, B) and one triple (A, B, C)
Ref:	=1987A&A...181..351H
by	HIGGS L.A. , VALLEE J.P., ALBINSON J.S., BATRLA W., GOSS W.M.
	Astron. Astrophys., 181, 351-364 (1987)
	Further observations of the peculiar galactic radio source BG 2107+49.
o	Table 4: <HVABG NNA> (Nos 1-42) with 7 double sources (A, B) and one triple (A, B, C)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HVB2017]
[HVB2017]	(Helmi+Veljanoski+Breddels+, 2017) (Not yet in Simbad)
Write:	<<[HVB2017] VelHel-N>>
N:	9
Object:	Stellar Stream (SIMBAD class: Stream = Stellar Stream)
Note:	N=9 overdensities in the nearby stellar halo. Use of Gaia DR1 TGAS and RAVE DR5 data.
Ref:	=2017A&A...598A..58H
by	HELMI A. , VELJANOSKI J., BREDDELS M.A., TIAN H., SALES L.V.
	Astron. Astrophys., 598A, 58-58 (2017)
	A box full of chocolates: The rich structure of the nearby stellar halo revealed by Gaia and RAVE.
o	Fig. 10: <[HVB2017] VelHel-N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HVB89]
[HVB89]	(Helfand+Velusamy+Becker+, 1989)
Write:	<<[HVB89] G28.60-0.13 A>> <<[HVB89] G28.60-0.13 A'>>
N:	9+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLA observations of the radio-source G28.60-0.13 = [ADP79] 28.600+0.126.
in source:	[ADP79] 028.600+0.126
Ref:	=1989ApJ...341..151H
by	HELFAND D.J. , VELUSAMY T., BECKER R.H., LOCKMAN F.J.
	Astrophys. J., 341, 151-162 (1989)
	The prevalence of supernova remnants among unidentified galactic radio sources.
o	Fig.6, Table 2: <[HVB89] G28.60-0.13 A> (Nos A-I), <[HVB89] G28.60-0.13 A'> (No. C').
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HVC
HVC	(High-Velocity Cloud)= (CHVC)
Write:	<<HVC LLL+BB+VVV>> <<HVC LLL.l+BB.b+VVV>> <<HVC LLL.l+BB+VVV>> <<HVC LLL.l+BB.b+VVV.v>>
Object:	HVC (SIMBAD class: HVCld = High-velocity Cloud)
Note:	Systematic designation. The term HVC is traditionally reserved for clouds having a velocity in excess of about 80km/s. See IVC, LVC. See [H71], [H75b], [MC79a], [M81c], [HW88b], [BCM89].
Details on Acronym: HVC
HVC	(High-Velocity Cloud)
*****	Avoid the usage of HVC, prefer WV
Origin	of the Acronym: L (1998AJ....116.1205S)
Details on Acronym: HVCS
HVCS	(Herschel Virgo Cluster Survey)
Write:	<<HVCS NNNN>>
N:	3102
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Herschel SPIRE observations at 250, 350 and 500µm, as part of the Herschel Virgo Cluster Survey (http://www.hevics.org/). Format NNNN: We cross-correlated the SPIRE catalogs with the SDSS DR10 survey.
Ref:	=2015A&A...573A.129P
by	PAPPALARDO C. , BENDO G.J., BIANCHI S., HUNT L., ZIBETTI S., CORBELLI E., DI SEREGO ALIGHIERI S., GROSSI M., DAVIES J., BAES M., DE LOOZE I., FRITZ J., POHLEN M., SMITH M.W.L., VERSTAPPEN J., BOQUIEN M., BOSELLI A., CORTESE L., HUGHES T., VIAENE S., BIZZOCCHI L., CLEMENS M.
	Astron. Astrophys., 573A, 129-129 (2015)
	The Herschel Virgo Cluster Survey. XVII. SPIRE point-source catalogs and number counts.
o	hevics.dat: <HVCS NNNN> (Nos 1-3102).
=E=	Catalogue in electronic form as J/A+A/573/A129
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HVF2005]
[HVF2005]	(Holden+Van der Wel+Franx+, 2006)
Write:	<<[HVF2005] NNNN>>
N:	4
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations of N=4 galaxies in RDCS J1252-2927.
in source:	RDCS J1252-2927
Ref:	=2005ApJ...620L..83H
by	HOLDEN B.P. , VAN DER WEL A., FRANX M., ILLINGWORTH G.D., BLAKESLEE J.P., VAN DOKKUM P., FORD H., MAGEE D., POSTMAN M., RIX H.-W., ROSATI P.
	Astrophys. J., 620, 83-86 (2005)
	The fundamental plane of cluster elliptical galaxies at z=1.25.
o	Fig.1 et Table 1: <[HVF2005] NNNN> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HVG2012]
[HVG2012]	(Hong+van den Berg+Grindlay+, 2012)
Write:	<<[HVG2012] LWP NN>>
N:	10 (SIMBAD class: CataclyV* = Cataclysmic Binary)
Note:	N=10 periodic X-ray sources from the 1 Ms Chandra ACIS observation of the Limiting Window (LW) region.
Ref:	=2012ApJ...746..165H
by	HONG J. , VAN DEN BERG M., GRINDLAY J.E., SERVILLAT M., ZHAO P.
	Astrophys. J., 746, 165 (2012)
	Discovery of a significant magnetic cataclysmic variable population in the limiting window.
o	Swift J1353.5-0127 is a misprint for Swift J1753.5-0127.
o	Table 2: <[HVG2012] LWP NN> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HVG94]
[HVG94]	(Hunter+Woerden+Gallagher, 1994)
Write:	<<[HVG94] NGC 1140 NN>> <<[HVG94] NGC 1800 N>> <<[HVG94] NGC 4670 NN>>
N:	18+8+11
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 6: radio-sources in NGC 1140, (Nos 1-18), format 'NGC 1140 NN'. radio-sources in NGC 1800, (Nos 1-8), format 'NGC 1800 N'. radio-sources in NGC 4670. (Nos 1-11), format 'NGC 4670 NN'.
in source:	NGC 1140
in source:	NGC 1800
in source:	NGC 4670
Ref:	=1994ApJS...91...79H
by	HUNTER D.A. , VAN WOERDEN H., GALLAGHER III J.S.
	Astrophys. J., Suppl. Ser., 91, 79-110 (1994)
	Neutral hydrogen and optical properties of three amorphous galaxies.
o	Table 6: <[HVG94] NGC 1140 NN> N=18, <[HVG94] NGC 1800 N> N=8, <[HVG94] NGC 4670 NN> N=11
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HVG99]
[HVG99]	(Hunter+Van Woerden+Gallagher, 1999)= ([HVG99a])
Write:	<<[HVG99] N-NNa>>
N:	18+19+7+30
Object:	(Rad) + HI (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Interferometric data of the galaxy NGC 4449. Table 3: format '3-NNa', N=18 continuum objects. Table 4: format '4-NN', N=19 HI shells. Table 5: format '5-N', N=7 HI Cloud Complexes. Table 6: format '6-NN', N=30 HI Clouds.
in source:	NGC 4449
Ref:	=1999AJ....118.2184H
by	HUNTER D.A. , VAN WOERDEN H., GALLAGHER J.S.
	Astron. J., 118, 2184-2210 (1999)
	Neutral hydrogen and star formation in the irregular galaxy NGC 4449.
o	Table 3: <[HVG99] 3-NNa> (Nos 3-1 to 3-13, 3-14a to 3-14b, 3-15 to 3-17). Table 4: <[HVG99] 4-NN> (Nos 4-1 to 4-19). Table 5: <[HVG99] 5-N> (Nos 5-1 to 5-7). Table 6: <[HVG99] 6-NN> (Nos 6-1 to 6-30).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HVG99a]
[HVG99a]	(Hunter+Van Woerden+Gallagher, 1999)
*****	Avoid the usage of [HVG99a], prefer [HVG99]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HVG99b]
[HVG99b]	(Huchra+Vogeley+Geller, 1999)
Write:	<<[HVG99b] HHMMm+DDMMA>> <<[HVG99b] HHMMm+DDMMW>> <<[HVG99b] AHHMM+DDMMA>>
N:	2968
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=2960 galaxies among the 4391 in the CfA2 survey. See [HGD90] for the NGP zone.
Ref:	=1999ApJS..121..287H
by	HUCHRA J.P. , VOGELEY M.S., GELLER M.J.
	Astrophys. J., Suppl. Ser., 121, 287-368 (1999)
	The CfA redshift survey: data for the South Galactic Cap.
o	Table 1: <[HVG99b] HHMMm+DDMMA>, <[HVG99b] HHMMm+DDMMW>, N=2943, <[HVG99b] AHHMM+DDMMA> N=25.
=E=	Catalogue in electronic form as J/ApJS/121/287
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HVH2010]
[HVH2010]	(Hammer+Verdoes Kleijn+Hoyos+, 2010)= (Coma)
Write:	<<[HVH2010] Comai JHHMMSS.sss+DDMMSS.ss>> <<[HVH2010] ComaiHHMSS.ssspDDMSS.ss>> (not recognised by Simbad, but found in literature)
N:	∼73000
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	The HST ACS Coma cluster survey. Deep imaging in the F475W and F814W passbands.
in source:	Coma Cluster = ACO 1656
Ref:	=2010ApJS..191..143H
by	HAMMER D. , VERDOES KLEIJN G., HOYOS C., DEN BROK M., BALCELLS M., FERGUSON H.C., GOUDFROOIJ P., CARTER D., GUZMAN R., PELETIER R.F., SMITH R.J., GRAHAM A.W., TRENTHAM N., PENG E., PUZIA T.H., LUCEY J.R., JOGEE S., AGUERRI A.L., BATCHELDOR D., BRIDGES T.J., CHIBOUCAS K., DAVIES J.I., DEL BURGO C., ERWIN P., HORNSCHEMEIER A., HUDSON M.J., HUXOR A., JENKINS L., KARICK A., KHOSROSHAHI H., KOURKCHI E., KOMIYAMA Y., LOTZ J., MARZKE R.O., MARINOVA I., MATKOVIC A., MERRITT D., MILLER B.W., MILLER N.A., MOBASHER B., MOUHCINE M., OKAMURA S., PERCIVAL S., PHILLIPPS S., POGGIANTI B.M., PRICE J., SHARPLES R.M., TULLY R.B., VALENTIJN E.
	Astrophys. J., Suppl. Ser., 191, 143-159 (2010)
	The HST/ACS Coma cluster survey. II. Data description and source catalogs.
o	<[HVH2010] Comai JHHMMSS.sss+DDMMSS.ss> N~73000.
=E=	Catalogue in electronic form as <J/ApJS/191/143/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HVH91]
[HVH91]	(Hawkins+Veron+Hunstead+, 1991)= (HM)
Write:	<<[HVH91] HHMM+DDd>>
N:	2
Object:	BL Lac (SIMBAD class: BLLac = BL Lac)
Stat:	is completely incorporated in Simbad
Ref:	=1991A&A...248..421H
by	HAWKINS M.R.S. , VERON P., HUNSTEAD R.W., BURGESS A.M.
	Astron. Astrophys., 248, 421-425 (1991)
	Two BL Lacertae objects discovered through their optical variability.
o	cross-id. with B7 and B24 not in SIMBAD. Not [H86b]
o	Table 2: MH use <[HVH91] HHMM-DDd> N=2
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HVK2000]
[HVK2000]	(Hulleman+Van Kerkwijk+Kulkarni, 2000)
Write:	<<[HVK2000] A>>
N:	3
Object:	* + Blue (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=3 objects in the error circle of 4U 0142+61. A = star, D and G = blue objects.
Ref:	=2000Natur.408..689H
by	HULLEMAN F. , VAN KERKWIJK M.H., KULKARNI S.R.
	Nature, 408, 689-692 (2000)
	An optical counterpart to the anomalous X-ray pulsar 4U 0142+61.
o	fig.2 : PG 1657-042 not identified (not in ref. 29)
o	Fig.1: <[HVK2000] A> (Nos A, D, G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HVK2004]
[HVK2004]	(Hulleman+Van Kerkwijk+Kulkarni, 2004)
Write:	<<[HVK2004] NNN>>
N:	42
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Keck observations. Table 3: N=43 stars in the field of 4U 0142+61, first object A = [HVK2000] A = 4U 0142+61, then 42 objects (Nos 102-143).
Ref:	=2004A&A...416.1037H
by	HULLEMAN F. , VAN KERKWIJK M.H., KULKARNI S.R.
	Astron. Astrophys., 416, 1037-1045 (2004)
	The Anomalous X-ray Pulsar 4U 0142+61: Variability in the infrared and a spectral break in the optical.
o	Table 3: object A = [HVK2000] A. Paragr.4: object A = [ICP2003] A. Table 4 : AXP CXOU J0110043.1-721134 is a misprint for CXOU J010043.1-721133 (=SMC AXP).
o	Table 3: <[HVK2004] NNN> (Nos 102-143).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HVK2009]
[HVK2009]	(Hunter+Valenti+Kotak+, 2009) (Not yet in Simbad)
Write:	<<[HVK2009] NN>>
N:	10
Object:	* (SIMBAD class: Star)
Note:	N=10 local standards in the field of SN 2007gr.
Ref:	=2009A&A...508..371H
by	HUNTER D.J. , VALENTI S., KOTAK R., MEIKLE W.P.S., TAUBENBERGER S., PASTORELLO A., BENETTI S., STANISHEV V., SMARTT S.J., TRUNDLE C., ARKHAROV A.A., BUFANO F., CAPPELLARO E., DI CARLO E., DOLCI M., ELIAS-ROSA N., FRANDSEN S., FYNBO J.U., HOPP U., LARIONOV V.M., LAURSEN P., MAZZALI P., NAVASARDYAN H., RIES C., RIFFESER A., RIZZI L., TSVETKOV D.Y., TURATTO M., WILKE S.
	Astron. Astrophys., 508, 371-389 (2009)
	Extensive optical and near-infrared observations of the nearby, narrow-lined type IC SN 2007gr: days 5 to 415.
o	Fig. 1, Table a.1: <[HVK2009] NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HVK87]
[HVK87]	(Hummel+van der Hulst+Keel, 1987) (Not yet in Simbad)
Write:	<<[HVK87] Em NN>> <<[HVK87] Background N>>
N:	10+5
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Fig.3, Table 4: N=10 regions of emission in the ring structure. Table 5: N=5 background radio-sources. See also [KRL2000].
in source:	NGC 1097
Ref:	=1987A&A...172...32H
by	HUMMEL E. , VAN DER HULST J.M., KEEL W.C.
	Astron. Astrophys., 172, 32-42 (1987)
	Circumnuclear star formation in the central region of the barred spiral galaxy NGC 1097.
o	Fig.3, Table 4: <[HVK87] Em NN> (Nos 1-10). Table 5: <[HVK87] Background N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HVL90]
[HVL90]	(Heydari-Malayeri+Van Drom+Leisy, 1990)
Write:	<<[HVL90] N83 B-N>>
N:	3
Object:	HII Blob (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	See also [HCD2001].
in source:	Magellanic Clouds:LMC:LHA 120-N 83B = LHA 120-N 83B
Ref:	=1990A&A...240..481H
by	HEYDARI-MALAYERI M. , VAN DROM E., LEISY P.
	Astron. Astrophys., 240, 481-486 (1990)
	A new high excitation compact HII blob in the Large Magellanic Cloud.
o	<[HVL90] N83 B-N> (No. B-1).
Ref:	=2001A&A...372..495H
by	HEYDARI-MALAYERI M. , CHARMANDARIS V., DEHARVENG L., ROSA M.R., SCHAERER D., ZINNECKER H.
	Astron. Astrophys., 372, 495-507 (2001)
	HST study of the LMC compact star-forming region N83B.
o	Fig.3: <[HVL90] N83 B-N> (Nos B-2, B-3). Table 3: <[HCD2001] N83B NN> (Nos 1-36).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HVP2001]
[HVP2001]	(Ho+Van Dyk+Peng+, 2001) (Not yet in Simbad)
Write:	<<[HVP2001] SN YYYYA A>> <<[HVP2001] SN YYYYAA A>>
N:	10+7+1+4+12+2+3+7+5+8
Object:	* (SIMBAD class: Star)
Note:	Stars in the field of 10 SN. Finding charts in Figs 1 to 10.
Ref:	=2001PASP..113.1349H
by	HO W.C.G. , VAN DYK S.D., PENG C.Y., FILIPPENKO A.V., LEONARD D.C., MATHESON T., TREFFERS R.R., RICHMOND M.W.
	Publ. Astron. Soc. Pac., 113, 1349-1364 (2001)
	BVRI photometry of supernovae.
o	Table 2: <[HVP2001] SN YYYYAA A> N=59.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HVS
HVS	(HyperVelocity Star)
*****	Avoid the usage of HVS, prefer [BGK2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HVS
HVS	(Herschel Virgo cluster Survey)
Write:	<<HVS JHHMMSS+DDMM.m>>
N:	133
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Catalog of N=133 500µm-risers, or sources with fluxes rising from 250µm to 500µm, in the Herschel Virgo Cluster Survey (HeViCS) field. These sources are potential z≥4 galaxies.
in source:	NAME Virgo Cluster
Ref:	=2018A&A...614A..33D
by	DONEVSKI D. , BUAT V., BOONE F., PAPPALARDO C., BETHERMIN M., SCHREIBER C., MAZYED F., ALVAREZ-MARQUEZ J., DUIVENVOORDEN S.
	Astron. Astrophys., 614A, 33-33 (2018)
	Towards a census of high-redshift dusty galaxies with Herschel. A selection of "500 µm-risers".
o	Table D.1: <HVS JHHMMSS+DDMM.m> N=133.
o	Fig.6 G09-8988 is H-ATLAS J090045.4+004125 in SIMBAD.
=E=	Catalogue in electronic form as <J/A+A/614/A33/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HVW99]
[HVW99]	(Hong+Venturi+Wan+, 1999) (Not yet in Simbad)
Write:	<<[HVW99] HHMM+DDd N>>
N:	23
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Table 3: N=23 components of N=11 radio-sources.
Ref:	=1999A&AS..134..201H
by	HONG X.Y. , VENTURI T., WAN T.S., JIANG D.R., SHEN Z.-Q., LIU X., NICOLSON G., UMANA G.
	Astron. Astrophys., Suppl. Ser., 134, 201-210 (1999)
	VLBI observations of 21 extragalactic radio sources. Search for superluminal sources in the mid-southern hemisphere.
o	Table 3: <[HVW99] HHMM+DDd N> N=23.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HVZ2013]
[HVZ2013]	(Hajduk+Van Hoof+Zijlstra, 2013)
Write:	<<[HVZ2013] variable N>> <<[HVZ2013] high pm star>>
N:	3
Object:	* (SIMBAD class: Star)
Stat.	in SIMBAD: [HVZ2013] high pm star not created
Note:	WHT 4.2-m telescope observations of N=3 stars in the field of CK Vul .
Ref:	=2013MNRAS.432..167H
by	HAJDUK M. , VAN HOOF P.A.M., ZIJLSTRA A.A.
	Mon. Not. R. Astron. Soc., 432, 167-175 (2013)
	CK Vul: evolving nebula and three curious background stars.
o	Fig. 7: <[HVZ2013] variable N> (Nos 1-2), <[HVZ2013] high pm star> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HW
HW	(Hodge+Wright)
Write:	<<HW NN>>
N:	86
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Note:	Identif. on the V charts of Hodge and Wright.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1974AJ.....79..858H
by	HODGE P.W. , WRIGHT F.W.
	Astron. J., 79, 858-859 (1974)
	Catalog of 86 new star clusters in the Small Magellanic Cloud.
o	Table II: <HW NN> (Nos 1-86)
Details on Acronym: HW
HW	(Hughes+Wouterloot)
*****	Avoid the usage of HW, prefer [HW84]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: HW
HW	(Hartl+Weinberger)
*****	Avoid the usage of HW, prefer HaWe
Origin	of the Acronym: L (1998ApJ...495..337D)
Details on Acronym: [HW2000]
[HW2000]	(Heithausen+Walter, 2000)
Write:	<<[HW2000] N>>
N:	4
Object:	Molecular Complex (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=4 complexes of molecular gas near NGC 3077.
Ref:	=2000A&A...361..500H
by	HEITHAUSEN A. , WALTER F.
	Astron. Astrophys., 361, 500-506 (2000)
	Extensive molecular gas in the tidal arms near NGC 3077 - birth of a dwarf galaxy?
o	Table 1: <[HW2000] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HW2002]
[HW2002]	(Hunter+Wilcots, 2002)
Write:	<<[HW2002] UGC 199 NN>> <<[HW2002] DDO 26 NN>>
N:	16+10
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Continuum sources near UGC 199 and DDO 26.
Ref:	=2002AJ....123.2449H
by	HUNTER D.A. , WILCOTS E.M.
	Astron. J., 123, 2449-2461 (2002)
	The distribution of atomic hydrogen around two irregular galaxies.
o	Table 3, Fig.1: <[HW2002] UGC 199 NN> (Nos 1-16). Table 4, Fig.7: <[HW2002] DDO 26 NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HW2003]
[HW2003]	(Higdon+Wallin, 2003)
Write:	<<[HW2003] SN>>
N:	2
Object:	HI (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	N=2 HI emission sources, companion candidates of NGC 1097.
Ref:	=2003ApJ...585..281H
by	HIGDON J.L. , WALLIN J.F.
	Astrophys. J., 585, 281-297 (2003)
	A minor-merger interpretation for NGC 1097's "jets".
o	Jets R1 to R4 = [WZ75] R1 to R4. In table 1, declination of NGC 1097A and of NGC 1097B are not correct.
o	Text: <[HW2003] SN> (Nos S1-S2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HW2012]
[HW2012]	(Howarth+Walborn, 2012)= (BAT99)
Write:	<<[HW2012] BAT99-NNa>>
N:	2
Object:	WR (SIMBAD class: WolfRayet* = Wolf-Rayet)
Stat:	is completely incorporated in Simbad
Note:	Anglo-Australian Telescope 2dF and AAOmega observations of N=2 Wolf-Rayet stars in the LMC.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2012MNRAS.426.1867H
by	HOWARTH I.D. , WALBORN N.R.
	Mon. Not. R. Astron. Soc., 426, 1867-1869 (2012)
	Two new Wolf-Rayet stars in the Large Magellanic Cloud.
o	Table 1: <[HW2012] BAT99-NNa> (Nos 5a, 15a).
Details on Acronym: [HW78]
[HW78]	(Hodge+Wright, 1978)
Write:	<<[HW78] VNN>>
N:	23
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	Format 'VNN' found in the literature (V for Variable star), the authors use the format 'NN'.
in source:	UGC 5470 = Leo I
Ref:	=1978AJ.....83..228H
by	HODGE P.W. , WRIGHT F.W.
	Astron. J., 83, 228-233 (1978)
	Variable stars in the Leo I dwarf galaxy.
o	<[HW78] VNN> N=23, format VNN found in litt., authors use the format NN
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HW84]
[HW84]	(Hughes+Wouterloot, 1984)= (HW)
Write:	<<[HW84] N>> <<[HW84] Na>> <<[HW84] N(WW)>> <<[HW84] N(r)>> <<[HW84] Na(r)>> <<[HW84] Na(WW)>>
N:	32
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	N=9 sources (Nos 1-9), with components 'Na', 'N(r)', or 'Na(r)' where 'r' stands for a minus roman digit. The authors add 2 other external components to 3d in 2001.
in source:	NAME Cep A
Ref:	=1984ApJ...276..204H
by	HUGHES V.A. , WOUTERLOOT J.G.A.
	Astrophys. J., 276, 204-210 (1984)
	The star-forming region in Cepheus A.
o	<[HW84] Na> N=14
Ref:	=1991ApJ...383..280H
by	HUGHES V.A.
	Astrophys. J., 383, 280-288 (1991)
	Time-dependent radio sources in the star-forming region Cepheus A (East).
o	<[HW84] N> (Nos 8, 9) added.
Ref:	=1993AJ....105..331H
by	HUGHES V.A.
	Astron. J., 105, 331-338 (1993)
	Is Cepheus A East a Herbig-Haro object?
o	Fig.2: <[HW84] 7c(r)> (Nos 7c(i), 7c(ii)).
Ref:	=1995MNRAS.272..469H
by	HUGHES V.A. , COHEN R.J., GARRINGTON S.
	Mon. Not. R. Astron. Soc., 272, 469-480 (1995)
	High-resolution observations of Cepheus A.
o	Table 2: <[HW84] 2(r)> (Nos 2(i), 2(ii)), <[HW84] 3d(r)> (Nos 3d(i), 3d(ii)).
Ref:	=1998ApJ...509..262T
by	TORRELLES J.M. , GOMEZ J.F., GARAY G., RODRIGUEZ L.F., CURIEL S., COHEN R.J., HO P.T.P.
	Astrophys. J., 509, 262-269 (1998)
	Systems with H_{2}O maser and 1.3 centimeter continuum emission in Cepheus A.
o	Table 1: <[HW84] Na(r)> (Nos 2(iii), 3d(iii), 3d(iv). Table 1: <[TGG98] Cep A VLA 1> N=1. Table 2: <[TGG98] HHMMSS.sss+DDMMSS.ss> N=39.
Ref:	=2001ApJ...563..919H
by	HUGHES V.A.
	Astrophys. J., 563, 919-927 (2001)
	The spectra of young protostars of Cepheus A.
o	<[HW84] Na(WW)> (Nos 3d(NW), 3d(SE)).
Ref:	=2006ApJ...638..878C
by	CURIEL S. , HO P.T.P., PATEL N.A., TORRELLES J.M., RODRIGUEZ L.F., TRINIDAD M.A., CANTO J., HERNANDEZ L., GOMEZ J.F., GARAY G., ANGLADA G.
	Astrophys. J., 638, 878-886 (2006)
	Large proper motions in the jet of the high-mass YSO Cepheus A HW2.
o	Fig.1: <[HW84] 2(WW)> (Nos 2(NE), 2(SW)) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HW84a]
[HW84a]	(Hughes+Wouterloot, 1984)
*****	Avoid the usage of [HW84a], prefer [HW84]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HW88]
[HW88]	(Hofmann+Weigelt, 1988)= ([HW88a])
Write:	<<[HW88] A>>
N:	4
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Fig.1: faint objects around the star Eta Car. [HW88] A = Eta Car itself. See also [WE86]
Ref:	=1988A&A...203L..21H
by	HOFMANN K.-H. , WEIGELT G.
	Astron. Astrophys., 203, 21-22 (1988)
	Speckle masking observation of η Carinae.
o	Fig.1: <[HW88] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HW88a]
[HW88a]	(Hofmann+Weigelt, 1988)
Note:	Fig.1: faint objects around the star Eta Car.
*****	Avoid the usage of [HW88a], prefer [HW88]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HW88b]
[HW88b]	(Hulsbosch+Wakker, 1988)
Write:	<<[HW88b] LLL+BB-VVV>>
N:	15
Object:	HVC (SIMBAD class: HVCld = High-velocity Cloud)
Stat:	is completely incorporated in Simbad
Note:	Table III: Selected newly discovered high-velocity clouds. See also HVC
Ref:	=1988A&AS...75..191H
by	HULSBOSCH A.N.M. , WAKKER B.P.
	Astron. Astrophys., Suppl. Ser., 75, 191-236 (1988)
	A deep, nearly complete, survey of northern high-velocity clouds.
o	Table I: N=8491 high velocity components, not in SIMBAD. Table IV: First column designation 'AA' not used in SIMBAD.
o	Table III: <[HW88b] LLL+BB-VVV> N=15.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HW94]
[HW94]	(Hunt+Whiteoak, 1994)
Write:	<<[HW94] H2O JHHMMSS.ss+DDMMSS.s>> <<[HW94] CO JHHMMSS.s+DDMMSS>> <<[HW94] N>>
N:	1+3+7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Australia Telescope Compact Array observations of the HII region LHA 120-N 159 in the LMC. N=1 H2O maser, N=3 CO concentrations, and N=7 radio emission features. The radio features are designated as 'N159A5' to 'N159A7' in 2006A&A...453..517T. See also [TLF2006].
in source:	Magellanic Clouds:LMC:LHA 120-N 159 = LHA 120-N 159
Ref:	=1994PASAu..11...68H
by	HUNT M.R. , WHITEOAK J.B.
	Proc. Astron. Soc. Australia, 11, 68-73 (1994)
	A second compact radio component detected in the LMC HII region N 159.
o	Table 1: <[HW94] H2O JHHMMSS.ss+DDMMSS.s> N=1, <[HW94] CO JHHMMSS.s+DDMMSS> N=3. Fig.1, Table 2: <[HW94] N> (Nos 1-5).
Ref:	=2006A&A...453..517T
by	TESTOR G. , LEMAIRE J.L., FIELD D., DIANA S.
	Astron. Astrophys., 453, 517-524 (2006)
	VLT/NACO near-infrared imaging and spectroscopy of N159A in the LMC HII complex N159.
o	Fig.1, Table 5: 'N159A5' to 'N159A7' = [HW94] 5 to 7 (not [HT82] objects).
o	Fig.1, Table 5: <[HW94] N> (Nos 6, 7) added. Tables 3, 5: <[TLF2006] NNNa> N=136+2 among (Nos 4-181, 121a, 123a).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HW95]
[HW95]	(Houghton+Whiteoak, 1995)
Write:	<<[HW95] NN>>
N:	11
Object:	CH3OH Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
in source:	NAME Sgr B2
Ref:	=1995MNRAS.273.1033H
by	HOUGHTON S. , WHITEOAK J.B.
	Mon. Not. R. Astron. Soc., 273, 1033-1040 (1995)
	The small-scale distribution of emission from the 6.7-GHz transition of methanol in Sgr B2.
o	Table 1: <[HW95] NN> (Nos 1-11)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HW97a]
[HW97a]	(Higdon+Wallin, 1997) (Not yet in Simbad)
Write:	<<[HW97a] CN>> <<[HW97a] NN>>
N:	2+54
Object:	G + HII (SIMBAD class: HIIReg = HII Region)
Note:	Fig.1: (Nos C1-C2), two companion galaxies to AM 0644-741. Table 2: (Nos 1-55), HII complexes in AM 0644-741
in source:	AM 0644-741
Ref:	=1997ApJ...474..686H
by	HIGDON J.L. , WALLIN J.F.
	Astrophys. J., 474, 686-700 (1997)
	Wheels of fire. III. Massive star formation in the ``Double-ringed'' ring galaxy AM 0644-741.
o	Fig.1: <[HW97a] CN> (Nos C1-C2). Table 2: <[HW97a] NN> (Nos 1-55).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HW97b]
[HW97b]	(Hobbs+Willmore, 1997)= (X)
Write:	<<[HW97b] N>>
N:	4
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations. N=4 X-ray sources in ACO 2670.
in source:	ACO 2670
Ref:	=1997MNRAS.289..685H
by	HOBBS I.S. , WILLMORE A.P.
	Mon. Not. R. Astron. Soc., 289, 685-692 (1997)
	A combined X-ray and optical analysis of the galaxy cluster A2670.
o	cD galaxy = [SEG88] 1. Table 4: sub-clusters = [B94] Clump A to D.
o	Fig.2: <[HW97b] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWB2008]
[HWB2008]	(Hughes+Wallerstein+Bossi, 2008)
Write:	<<[HWB2008] NNN>>
N:	165
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Apache Point Observatory 3.5m telescope observations of the central region of Bootes I.
in source:	Bootes DSph Galaxy = Bootes I
Ref:	=2008AJ....136.2321H
by	HUGHES J. , WALLERSTEIN G., BOSSI A.
	Astron. J., 136, 2321-2331 (2008)
	The age and metallicity of the Bootes I system.
o	Table 2: <[HWB2008] NNN> (Nos 1-165).
=E=	Catalogue in electronic form as <J/AJ/136/2321/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 1HWC
1HWC	(HAWC gamma-ray observatory, partial array data)
Write:	<<1HWC JHHMM+DDda>>
N:	20
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	The High-Altitude Water Cherenkov Gamma-Ray observatory is an all-sky surveying TeV detector. http://www.hawc-observatory.org/ This is the list of gamma-ray sources seen from the Pass 1 analysis. The letter "a" is for flagging sources with pre-trials significance >5 sigma but are <5 sigma after accounting for trials. We consider these candidate sources that may become more significant with additional data. We anticipate additional releases with more data and more sensitive analysis in the future following similar convention, e.g. 2HWC, and will include cross-identification tables with the analysis passes and other gamma-ray instruments.
Notes:	The HAWC array was completed in March 2015 and we anticipate additional release with more data and more sensitive analysis in the future following similar convention, e.g. 2HWC.
Auth.:	C. Michelle Hui Michigan Technological University
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: 2HWC
2HWC	(HAWC Observatory catalog)
Write:	<<2HWC JHHMM+DDd>>
N:	40 (SIMBAD class: gamma = Gamma-ray Source)
Note:	2HWC is the first catalog of TeV gamma-ray sources realized with the full HAWC instrument (http://www.hawc-observatory.org/), which is about to be submitted. Joint paper with other experiments should follow.
Notes:	J2000 coordinates follow the truncation rule.
Ref:	=2017ApJ...843...40A
by	ABEYSEKARA A.U. , ALBERT A., ALFARO R., ALVAREZ C., ALVAREZ J.D., ARCEO R., ARTEAGA-VELAZQUEZ J.C., AYALA SOLARES H.A., BARBER A.S., BAUGHMAN B., BAUTISTA-ELIVAR N., BECERRA GONZALEZ J., BECERRIL A., BELMONT-MORENO E., BENZVI S.Y., BERLEY D., BERNAL A., BRAUN J., BRISBOIS C., CABALLERO-MORA K.S., CAPISTRAN T., CARRAMINANA A., CASANOVA S., CASTILLO M., COTTI U., COTZOMI J., COUTINO DE LEON S., DE LA FUENTE E., DE LEON C., DIAZ HERNANDEZ R., DINGUS B.L., DUVERNOIS M.A., DIAZ-VELEZ J.C., ELLSWORTH R.W., ENGEL K., FIORINO D.W., FRAIJA N., GARCIA-GONZALEZ J.A., GARFIAS F., GERHARDT M., GONZALEZ MUNOZ A., GONZALEZ M.M., GOODMAN J.A., HAMPEL-ARIAS Z., HARDING J.P., HERNANDEZ S., HERNANDEZ-ALMADA A., HINTON J., HUI C.M., HUNTEMEYER P., IRIARTE A., JARDIN-BLICQ A., JOSHI V., KAUFMANN S., KIEDA D., LARA A., LAUER R.J., LEE W.H., LENNARZ D., LEON VARGAS H., LINNEMANN J.T., LONGINOTTI A.L., LUIS RAYA G., LUNA-GARCIA R., LOPEZ-COTO R., MALONE K., MARINELLI S.S., MARTINEZ O., MARTINEZ-CASTELLANOS I., MARTINEZ-CASTRO J., MARTINEZ-HUERTA H., MATTHEWS J.A., MIRANDA-ROMAGNOLI P., MORENO E., MOSTAFA M., NELLEN L., NEWBOLD M., NISA M.U., NORIEGA-PAPAQUI R., PELAYO R., PRETZ J., PEREZ-PEREZ E.G., REN Z., RHO C.D., RIVIERE C., ROSA-GONZALEZ D., ROSENBERG M., RUIZ-VELASCO E., SALAZAR H., SALESA GREUS F., SANDOVAL A., SCHNEIDER M., SCHOORLEMMER H., SINNIS G., SMITH A.J., SPRINGER R.W., SURAJBALI P., TABOADA I., TIBOLLA O., TOLLEFSON K., TORRES I., UKWATTA T.N., VIANELLO G., VILLASENOR L., WEISGARBER T., WESTERHOFF S., WISHER I.G., WOOD J., YAPICI T., YOUNK P.W., ZEPEDA A., ZHOU H.
	Astrophys. J., 843, 40-40 (2017)
	The 2HWC HAWC Observatory γ-ray catalog.
o	Tables 2-3: <2HWC JHHMM+DDd> N=40. University of Maryland
=E=	Catalogue in electronic form as <J/ApJ/843/40/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [HWC2006]
[HWC2006]	(Heinke+Wijnands+Cohn+, 2006)= (CX)
Write:	<<[HWC2006] CX NN>>
N:	50
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of the cluster Terzan 5. See also CXOGlb.
in source:	Cl Terzan 5
Ref:	=2006ApJ...651.1098H
by	HEINKE C.O. , WIJNANDS R., COHN H.N., LUGGER P.M., GRINDLAY J.E., POOLEY D., LEWIN W.H.G.
	Astrophys. J., 651, 1098-1111 (2006)
	Faint X-ray sources in the globular cluster Terzan 5.
o	Table 1, col(1): <[HWC2006] CX NN> (Nos 1-50) = Table 1, col(2): <CXOGlb JHHMMSS.s+DDMMSS> N=50.
=E=	Catalogue in electronic form as J/ApJ/651/1098
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 3HWC
3HWC	(Third HAWC Observatory Catalog)
Write:	<<3HWC JHHMM+DDd>>
N:	about 65 (SIMBAD class: gamma = Gamma-ray Source)
Note:	3HWC is the third catalog of TeV gamma-ray sources realized with the HAWC observatory (http://www.hawc-observatory.org/), to be submitted shortly. It is a followup to the 2HWC survey (https://data.hawc-observatory.org/datasets/2hwc-survey/catalog.php). See also 1HWC and 2HWC.
Ref:	=2020ApJ...905...76A
by	ALBERT A. , ALFARO R., ALVAREZ C., ANGELES CAMACHO J.R., ARTEAGA-VELAZQUEZ J.C., ARUNBABU K.P., AVILA ROJAS D., AYALA SOLARES H.A., BAGHMANYAN V., BELMONT-MORENO E., BENZVI S.Y., BRISBOIS C., CABALLERO-MORA K.S., CAPISTRAN T., CARRAMINANA A., CASANOVA S., COTTI U., COUTINO DE LEON S., DE LA FUENTE E., DIAZ HERNANDEZ R., DIAZ-CRUZ L., DINGUS B.L., DUVERNOIS M.A., DUROCHER M., DIAZ-VELEZ J.C., ELLSWORTH R.W., ENGEL K., ESPINOZA C., FAN K.L., FANG K., FERNANDEZ ALONSO M., FLEISCHHACK H., FRAIJA N., GALVAN-GAMEZ A., GARCIA D., GARCIA-GONZALEZ J.A., GARFIAS F., GIACINTI G., GONZALEZ M.M., GOODMAN J.A., HARDING J.P., HERNANDEZ S., HINTON J., HONA B., HUANG D., HUEYOTL-ZAHUANTITLA F., HUNTEMEYER P., IRIARTE A., JARDIN-BLICQ A., JOSHI V., KIEDA D., LARA A., LEE W.H., LEON VARGAS H., LINNEMANN J.T., LONGINOTTI A.L., LUIS-RAYA G., LUNDEEN J., LOPEZ-COTO R., MALONE K., MARANDON V., MARTINEZ O., MARTINEZ-CASTELLANOS I., MARTINEZ-CASTRO J., MATTHEWS J.A., MIRANDA-ROMAGNOLI P., MORALES-SOTO J.A., MORENO E., MOSTAFA M., NAYERHODA A., NELLEN L., NEWBOLD M., NISA M.U., NORIEGA-PAPAQUI R., OLIVERA-NIETO L., OMODEI N., PEISKER A., PEREZ ARAUJO Y., PEREZ-PEREZ E.G., REN Z., RHO C.D., RIVIERE C., ROSA-GONZALEZ D., RUIZ-VELASCO E., SALAZAR H., SALESA GREUS F., SANDOVAL A., SCHNEIDER M., SCHOORLEMMER H., SERNA F., SINNIS G., SMITH A.J., SPRINGER R.W., SURAJBALI P., TOLLEFSON K., TORRES I., TORRES-ESCOBEDO R., UKWATTA T.N., URENA-MENA F., WEISGARBER T., WERNER F., WILLOX E., ZEPEDA A., ZHOU H., DE LEON C., ALVAREZ J.D., (The HAWC Collaboration)
	Astrophys. J., 905, 76-76 (2020)
	3HWC: the third HAWC catalog of very-high-energy γ-ray sources.
o	Table 1: <3HWC JHHMM+DDd> N=65. Michigan State University
=E=	Catalogue in electronic form as <J/ApJ/905/76/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [HWC86]
[HWC86]	(Hilton+White+Cronin+, 1986)
Write:	<<[HWC86] N>>
N:	3
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	LDN 379
Ref:	=1986A&A...154..274H
by	HILTON J. , WHITE G.J., CRONIN N.J., RAINEY R.
	Astron. Astrophys., 154, 274-278 (1986)
	Lynds 379 : a new source of bipolar molecular flow.
o	Table 1: <[HWC86] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWC97]
[HWC97]	(Hill+Waller+Cornett+, 1997)
Write:	<<[HWC97] NN>>
N:	28
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	UIT observations aboard the Astro-2 Spacelab mission
in source:	M 51 = NGC 5194
Ref:	=1997ApJ...477..673H
by	HILL J.K. , WALLER W.H., CORNETT R.H., BOHLIN R.C., CHENG K.-P., NEFF S.G., O'CONNELL R.W., ROBERTS M.S., SMITH A.M., HINTZEN P.M.N., SMITH E.P., STECHER T.P.
	Astrophys. J., 477, 673-678 (1997)
	Ultraviolet colors and extinctions of H II regions in the Whirlpool galaxy (M51).
o	Table 2, col(2): numbering from Rand, 1995, private comm., not in SIMBAD
o	Table 2, col(1): <[HWC97] NN> (Nos 1-28)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWC99]
[HWC99]	(Hunt+Whiteoak+Cragg+, 1999)
Write:	<<[HWC99] N>>
N:	7
Object:	Peak (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	ATCA observations of HC3N. Table 1: numbers (Nos 1-7) have been assigned to positions near continuum maxima, letters to other selected positions with faint or undetectable continuum emission (letters are not corresponding to objects).
in source:	NAME Sgr B2
Ref:	=1999MNRAS.302....1H
by	HUNT M.R. , WHITEOAK J.B., CRAGG D.M., WHITE G.L., JONES P.A.
	Mon. Not. R. Astron. Soc., 302, 1-8 (1999)
	High-resolution observations of the j=1-0 transition of cyanoacetylene in Sgr B2.
o	calibrators not in SIMBAD
o	Table 1: <[HWC99] N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWE2003]
[HWE2003]	(Hancock+Weistrop+Eggers+, 2003)
Write:	<<[HWE2003] NGC 3395 NN>> <<[HWE2003] NGC 3396 NN>>
N:	66+51
Object:	(Far UV) (SIMBAD class: UV = UV-emission Source)
Note:	HST STIS observations of the 2 interacting galaxies NGC 3395 and NGC 3396. N=66 FUV knots in NGC 3395, and N=51 FUV knots in NGC 3396.
in source:	NGC 3395
in source:	NGC 3396
Ref:	=2003AJ....125.1696H
by	HANCOCK M. , WEISTROP D., EGGERS D., NELSON C.H.
	Astron. J., 125, 1696-1710 (2003)
	Star-forming knots in the UV-bright interacting galaxies NGC 3395 and NGC 3396.
o	Table 2: <[HWE2003] NGC 3395 NN> (Nos 1-66). Table 3: <[HWE2003] NGC 3396 NN> (Nos 1-51).
=E=	Catalogue in electronic form as J/AJ/125/1696
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWE99]
[HWE99]	(Hardin+Walton+Ellis+, 1999)
Write:	<<[HWE99] JHHMMSS.ss+DDMMSS.s>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxy of SN 1999cj and SN 1999ck
Ref:	=1999IAUC.7182Q...1H
by	HARDIN D. , WALTON N.A., ELLIS R.S., IRWIN M., McMAHON R.G., HOOK I., RUIZ-LAPUENTE P., MENDEZ J., VISCO A., ASTIER P., BALLAND C., BLANC G., BLANCHARD A., FABBRO S., HAMMER F., LETESSIER-SELVON A., LEVY J.-M., MOUCHET M., PAIN R., RICH J., SHAHMANECHE K., TAILLET R.
	IAU Circ., 7182, 1-None (1999)
	Supernovae 1999cj and 1999ck in anonymous galaxies.
o	<[HWE99] JHHMMSS.ss+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWF2003]
[HWF2003]	(Holland+Weidinger+Finbo+, 2003)
Write:	<<[HWF2003] A>>
N:	7
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	NOT observations of N=7 secondary standard stars in the field of GRB 021004.
Ref:	=2003AJ....125.2291H
by	HOLLAND S.T. , WEIDINGER M., FYNBO J.P.U., GOROSABEL J., HJORTH J., PEDERSEN K., ALVAREZ J.M., AUGUSTEIJN T., CASTRO CERON J.M., CASTRO-TIRADO A., DAHLE H., EGHOLM M.P., JAKOBSSON P., JENSEN B.L., LEVAN A., MOLLER P., PEDERSEN H., PURSIMO T., RUIZ-LAPUENTE P., THOMSEN B.
	Astron. J., 125, 2291-2298 (2003)
	Optical photometry of GRB 021004: the first month.
o	Fig.1, Table 1: <[HWF2003] A> (Nos A-G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWF2005]
[HWF2005]	(Haarsma+Winn+Falco+, 2005)
Write:	<<[HWF2005] JHHMMSS.ss+DDMMSS.s>>
N:	32
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Identification of radio lobes in FIRST images. See also FOV.
Ref:	=2005AJ....130.1977H
by	HAARSMA D.B. , WINN J.N., FALCO E.E., KOCHANEK C.S., AMMAR P., BOERSMA C., FOGWELL S., MUXLOW T.W.B., McLEOD B.A., LEHAR J.
	Astron. J., 130, 1977-1995 (2005)
	The FIRST-Optical-VLA survey for lensed radio lobes.
o	Table 1: <FOV JHHMM+DDMM> N=92. Table 2: <FOV JHHMM+DDMM W> N=5. Table 2, cols(2, 3): <[HWF2005] JHHMMSS.ss+DDMMSS.s> N=32.
=E=	Catalogue in electronic form as J/AJ/130/1977
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWG2018]
[HWG2018]	(Heyer+Wilson+Gutermuth+, 2018)
Write:	<<[HWG2018] AzTEC NNNN>> <<[HWG2018] LMT GLLL.lll+BB.bbb>> <<[HWG2018] LMT_LLL.lll+BB.bbb>> (not recognised by Simbad, but found in literature)
N:	1545*2
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Large Millimeter Telescope (LMT) AzTEC 1.1mm observations of N=1545 compact sources from a 1 square degree area within the Galactic Plan.
Ref:	=2018MNRAS.473.2222H
by	HEYER M. , WILSON G.W., GUTERMUTH R., LIZANO S., GOMEZ-RUIZ A., KURTZ S., LUNA A., SERRANO BERNAL E.O., SCHLOERB F.P.
	Mon. Not. R. Astron. Soc., 473, 2222-2233 (2018)
	Early science with the large millimetre telescope: fragmentation of molecular clumps in the galaxy.
o	Table 1, col(1): <[HWG2018] AzTEC NNNN> (Nos 1-1545) = Table 1, col(2): <[HWG2018] LMT GLLL.lll+BB.bbb> N=1545.
=E=	Catalogue in electronic form as <J/MNRAS/473/2222/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWH2009]
[HWH2009]	(Haas+Willner+Heymann+, 2009)
Write:	<<[HWH2009] NN>>
N:	29
Object:	G (SIMBAD class: Galaxy)
Note:	Spitzer MIPS/IRAC and MMT MegaCam/SWIRC observations of the quasar 3C 270.1.
Ref:	=2009ApJ...695..724H
by	HAAS M. , WILLNER S.P., HEYMANN F., ASHBY M.L.N., FAZIO G.G., WILKES B.J., CHINI R., SIEBENMORGEN R., STERN D.
	Astrophys. J., 695, 724-731 (2009)
	Clustering of red galaxies around the z = 1.53 quasar 3C 270.1.
o	Table 1: <[HWH2009] NN> (Nos 1-29).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWH2014]
[HWH2014]	(Huang+Wu+Hui+, 2014)
Write:	<<[HWH2014] NN>>
N:	21
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-I observations of N=21 X-ray sources in the field of the Galactic supernova remnant candidate G38.7-1.4.
in source:	GAL 038.7-01.4
Ref:	=2014ApJ...785..118H
by	HUANG R.H.H. , WU J.H.K., HUI C.Y., SEO K.A., TREPL L., KONG A.K.H.
	Astrophys. J., 785, 118 (2014)
	Identification campaign of supernova remnant candidates in the Milky Way. II. X-ray studies of G38.7-1.4.
o	Table 1: <[HWH2014] NN> N=21.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWI2021]
[HWI2021]	(Hu+Wang+Infante+, 2021) (Not yet in Simbad)
Write:	<<[HWI2021] LAGER-z7OD1>> <<[HWI2021] LAE-NN>>
N:	1+21
Object:	Protocluster + LAE (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	CTIO DECam, Magellan IMACS and LDSS3 observations of N=21 Lyman Alpha Emitters, including 16 members of N=1 protocluster at z=6.9, as part of the Lyman Alpha Galaxies in the Epoch of Reionization (LAGER) project. See also [ZWR2017], [YIR2019], [HWZ2019].
in source:	NAME COSMOS Field
Ref:	=2021NatAs...5..485H
by	HU W. , WANG J., INFANTE L., RHOADS J.E., ZHENG Z.-Y., YANG H., MALHOTRA S., BARRIENTOS L.F., JIANG C., GONZALEZ-LOPEZ J., PRIETO G., PEREZ L.A., HIBON P., GALAZ G., COUGHLIN A., HARISH S., KONG X., KANG W., KHOSTOVAN A.A., PHARO J., VALDES F., WOLD I., WALKER A.R., ZHENG X.
	NatAs, 5, 485-490 (2021)
	A Lyman-α protocluster at redshift 6.9.
o	<[HWI2021] LAGER-z7OD1> N=1. Suppl. Table 1: <[HWI2021] LAE-NN> (Nos 1-21).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [HWJ2019]
[HWJ2019]	(Hale+Williams+Jarvis+, 2019) (Not yet in Simbad)
Write:	<<[HWJ2019] JHHMMSS.ss+DDMMSS.s>>
N:	3044
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	LOFAR 120-168MHz observations of N=3044 sources in the XMM Large-Scale Structure (XMM-LSS) field.
in source:	NAME XMM-LSS Field
Ref:	=2019A&A...622A...4H
by	HALE C.L. , WILLIAMS W., JARVIS M.J., HARDCASTLE M.J., MORABITO L.K., SHIMWELL T.W., TASSE C., BEST P.N., HARWOOD J.J., HEYWOOD I., PRANDONI I., ROTTGERING H.J.A., SABATER J., SMITH D.J.B., VAN WEEREN R.J.
	Astron. Astrophys., 622A, 4-4 (2019)
	LOFAR observations of the XMM-LSS field.
o	lxmmmerg: <[HWJ2019] JHHMMSS.ss+DDMMSS.s> N=3044.
=E=	Catalogue in electronic form as <J/A+A/622/A4/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWJ84]
[HWJ84]	(Harvey+Wilking+Joy, 1984)= (FIRS)
Write:	<<[HWJ84] FIRS N>>
N:	2
Object:	(Far IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	'FIRS 1' is in Sh 2-68. 'FIRS 2', '3', '4' are in NGC 7129. See also [SB86] S68
in source:	SH 2-68
in source:	NGC 7129
Ref:	=1984ApJ...278..156H
by	HARVEY P.M. , WILKING B.A., JOY M.
	Astrophys. J., 278, 156-169 (1984)
	Infrared observations of dust cloud structure in young R associations: NGC 1333, S 68 and NGC 7129.
o	Table 2: <[HWJ84] FIRS N> (Nos 1-2)
Ref:	=1998A&A...335..243E
by	EIROA C. , PALACIOS J., CASALI M.M.
	Astron. Astrophys., 335, 243-247 (1998)
	NGC 7129 FIRS 2: an intermediate-mass counterpart of Class 0 objects.
o	p. 246 : IRAS 20050 = IRAS 20050+2720
o	Table 2: <[HWJ84] FIRS N> (Nos 3-4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWJ85]
[HWJ85]	(Harvey+Wilking+Joy, 1984)= (IRS)
Write:	<<[HWJ85] NNW>>
N:	13
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Map in Fig.1
in source:	NAME GGD 12-15
Ref:	=1985ApJ...288..725H
by	HARVEY P.M. , WILKING B.A., JOY M., LESTER D.F.
	Astrophys. J., 288, 725-730 (1985)
	An infrared study of the bipolar outflow region GGD 12-15.
o	Table 2: <[HWJ85] NNW> (Nos 1-8, 9E, 9M, 10-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWK2001]
[HWK2001]	(Hoard+Wachter+Kim-Quijano, 2001) (Not yet in Simbad)
Write:	<<[HWK2001] N>>
N:	9
Object:	* (SIMBAD class: Star)
Note:	N=9 comparison stars in the field of 'NAME Phoenix 1'.
Ref:	=2001PASP..113..482H
by	HOARD D.W. , WACHTER S., KIM-QUIJANO J.
	Publ. Astron. Soc. Pac., 113, 482-489 (2001)
	Optical photometry of the double-lined cataclysmic variable Phoenix 1.
o	Fig.1, Table 2: <[HWK2001] N> (Nos 1-9).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWK2003]
[HWK2003]	(Hardcastle+Worrall+Kraft+, 2003)
Write:	<<[HWK2003] SJN>> <<[HWK2003] SNA>>
N:	3+4
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 8.4GHz observations of Cen A. N=3 inner counterjet knots (Nos SJ1 to SJ3), and knots S1 and S2 (= [CBF86] SL1 and [CBF86] SL2), knot S2 is divided in 2 sub-knots A and B. See also BGLO, [CBF86], [KFJ2002].
in source:	Cen A = NGC 5128
Ref:	=2003ApJ...593..169H
by	HARDCASTLE M.J. , WORRALL D.M., KRAFT R.P., FORMAN W.R., JONES C., MURRAY S.S.
	Astrophys. J., 593, 169-183 (2003)
	Radio and X-ray observations of the jet in Centaurus A.
o	The knots designated as 'S1' and 'S2' in Fig.1 and in the text are [CBF86] SL1 and [CBF86] SL2 in SIMBAD ('SL1' and 'SL2' in 1992ApJ...395..444C).
o	Fig.1: <BGLO Cen A Knot ANa> (Nos A2a, A3a, A3b, A5a, A6a, B1a) added. Fig.1: <[HWK2003] SJN> (Nos SJ1 to SJ3), <[HWK2003] SNA> (Nos S1-S2, S2A, S2B). Fig.5: <[KFJ2002] AXNA> (Nos AX1A, AX1C, SX1, SX2A, SX2B) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWK96]
[HWK96]	(Hambly+Wood+Keenan+, 1996)
Write:	<<[HWK96] 603-NNN>>
N:	16
Object:	* (SIMBAD class: Star)
Note:	Spectroscopy from UBR Schmidt Telescope plates in U.K. Telescope survey field 603. N=16 among (Nos 2-139)
Ref:	=1996A&A...306..119H
by	HAMBLY N.C. , WOOD K.D., KEENAN F.P., KILKENNY D., DUFTON P.L., MILLER L., GILMORE G., IRWIN M.J., TOTTEN E.J.
	Astron. Astrophys., 306, 119-124 (1996)
	A search for star formation around the Galactic halo B-type star PHL 346.
o	Tables 2, 3, 4: <[HWK96] 603-NNN> N=16 among (Nos 2-139)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWL2007]
[HWL2007]	(Houck+Weedman+Le Floc'h+, 2007)= (SST24)
Write:	<<[HWL2007] NN>> <<[HWL2007] SST24 JHHMMSS.ss+DDMMSS.s>>
N:	50
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spitzer Space Telescope NDWFS observations of a region in Bootes. See also [HSW2005], [WLH2006], [WSH2006].
Ref:	=2007ApJ...671..323H
by	HOUCK J.R. , WEEDMAN D.W., LE FLOC'H E., HAO L.
	Astrophys. J., 671, 323-332 (2007)
	Spitzer spectra of a 10 mJy galaxy sample and the star formation rate in the Local universe.
o	Table 1: <[HWL2007] NN> (Nos 1-50) = <[HWL2007] SST24 JHHMMSS.ss+DDMMSS.s> N=50.
=E=	Catalogue in electronic form as J/ApJ/671/323
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWL2009]
[HWL2009]	(Habersetl+Williger+Lauroesch+, 2009)
Write:	<<[HWL2009] LQG JHHMMSS+DDMMSS>>
N:	462
Object:	LBG (SIMBAD class: Galaxy)
Note:	GALEX observations of Lyman Break Galaxies from the Clowes-Campusano LQG (Large Quasar Group) survey. Use of SDSS data.
Ref:	=2009ApJ...702..506H
by	HABERZETTL L. , WILLIGER G.M., LAUROESCH J.T., HAINES C.P., VALLS-GABAUD D., HARRIS K.A., KOEKEMOER A.M., LOVEDAY J., CAMPUSANO L.E., CLOWES R.G., DAVE R., GRAHAM M.J., SOCHTING I.K.
	Astrophys. J., 702, 506-522 (2009)
	The Clowes-Campusano Large Quasar Group Survey. I. GALEX selected sample of Lyman break galaxies at z ~ 1.
o	Table 2: <[HWL2009] LQG JHHMMSS+DDMMSS> N=462.
=E=	Catalogue in electronic form as <J/ApJ/702/506/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWL2018]
[HWL2018]	(Hu+Wang+Lin+, 2018) (Not yet in Simbad)
Write:	<<[HWL2018] NN>>
N:	15
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	MMT 6.5m telescope Hectospec and NAOC 2.16m telescope observations of N=15 HII regions in the nearby galaxy M101.
in source:	NGC 5457 = M 101
Ref:	=2018ApJ...854...68H
by	HU N. , WANG E., LIN Z., KONG X., CHENG F., FAN Z., FANG G., LIN L., MAO Y., WANG J., ZHOU X., ZHOU Z., ZHU Y., ZOU H.
	Astrophys. J., 854, 68-68 (2018)
	M101: spectral observations of H II regions and their physical properties.
o	Table 1: <[HWL2018] NN> (Nos 1-15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWL94]
[HWL94]	(Higgs+Wendker+Landecker, 1994)
Write:	<<[HWL94] 2-N>> <<[HWL94] 3-N>> <<[HWL94] 4-N>> <<[HWL94] a>> <<[HWL94] A>>
N:	8+4+2+5+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Table 2: 1.496GHz sources, format '2-N', N=8. Table 3: 4.86GHz sources, format '3-N', N=4. Table 4: 8.44GHz sources, format '4-N', N=2, cross-id. with sources A and B. Table 5: N=6 stars. Format 'a' and 'A', (Nos a-e) N=5, and source A.
in source:	GRS 079.29 +00.46
Ref:	=1994A&A...291..295H
by	HIGGS L.A. , WENDKER H.J., LANDECKER T.L.
	Astron. Astrophys., 291, 295-309 (1994)
	G 79.29+0.46: a young stellar-wind shell in Cygnus X.
o	Table 2: <[HWL94] 2-N> N=8, Table 3: <[HWL94] 3-N> N=4, Table 4: <[HWL94] 4-N> N=2, Table 5: <[HWL94] a> N=5, <[HWL94] A> N=2
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWM2000]
[HWM2000]	(Hasegawa+Wakamatsu+Malkan+, 2000)= (Oph)
Write:	<<[HWM2000] R>> <<[HWM2000] Oph JHHMMSS+DDMM>>
N:	7+218
Object:	Cluster of G + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table 4: N=7 new clumps in the sky distribution of galaxies in the Ophiuchus region. Table C1: N=219 galaxies.
in source:	NAME Ophiuchus Region
Ref:	=2000MNRAS.316..326H
by	HASEGAWA T. , WAKAMATSU K.-I., MALKAN M., SEKIGUCHI K., MENZIES J.W., PARKER Q.A., JUGAKU J., KAROJI H., OKAMURA S.
	Mon. Not. R. Astron. Soc., 316, 326-344 (2000)
	Large-scale structure of galaxies in the Ophiuchus region.
o	Table 4: <[HWM2000] R> (Nos II-VIII). Table C1: <[HWM2000] Oph JHHMMSS+DDMM> N=218.
=E=	Catalogue in electronic form as J/MNRAS/316/326
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWM2022]
[HWM2022]	(Harish+Wold+Malhotra+, 2022) (Not yet in Simbad)
Write:	<<[HWM2022] JHHMMSS+DDMMSS>>
N:	21
Object:	Poss. LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	Keck I LRIS observations of N=21 LAE candidates in the COSMOS and WIDE12 fields, as part of the Lyman Alpha Galaxies in the Epoch of Reionization (LAGER) project. See also [ZWR2019], [YIR2019], HWZ2019], [HWI2021].
in source:	NAME COSMOS Field
Ref:	=2022ApJ...934..167H
by	HARISH S. , WOLD I.G.B., MALHOTRA S., RHOADS J.E., HU W., WANG J., ZHENG Z.-Y., BARRIENTOS L.F., GONZALEZ-LOPEZ J., PEREZ L.A., KHOSTOVAN A.A., INFANTE L., JIANG C., MOYA-SIERRALTA C., PHARO J., VALDES F., YANG H.
	Astrophys. J., 934, 167 (2022)
	New Spectroscopic Confirmations of Lyα Emitters at Z ~ 7 from the LAGER Survey.
o	Table 2: <[HWM2022] JHHMMSS+DDMMSS> N=21.
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [HWM96]
[HWM96]	(Holtzman+Watson+Mould, 1996)= (Holtz) (Not yet in Simbad)
Write:	<<[HWM96] NGC NNNN NN>> <<[HWM96] ACO NNNN NN>>
N:	72+73+39+27+11+11
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
in source:	NGC 3597
in source:	NGC 6052
in source:	ACO 496
in source:	ACO 1795
in source:	ACO 2029
in source:	ACO 2597
Ref:	=1996AJ....112..416H
by	HOLTZMAN J.A. , WATSON A.M., MOULD J.R., GALLAGHER III J.S., BALLESTER G.E., BURROWS C.J., CLARKE J.T., CRISP D., EVANS R.W., GRIFFITHS R.E., HESTER J.J., HOESSEL J.G., SCOWEN P.A., STAPELFELDT K.R., TRAUGER J.T., WESTPHAL J.A.
	Astron. J., 112, 416-430 (1996)
	Star clusters in interacting and cooling flow galaxies.
o	Table 4: <[HWM96] NGC 3597 NN> (Nos 1-72). Table 5: <[HWM96] NGC 6052 NN> (Nos 1-73). Table 6: <[HWM96] ACO 496 NN> (Nos 1-39). Table 7: <[HWM96] ACO 1795 NN> N=27 among (Nos 2-30). Table 8: <[HWM96] ACO 2029 NN> N=11 among (Nos 3-17). Table 9: <[HWM96] ACO 2597 NN> N=11 among (Nos 1-14)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWN2006]
[HWN2006]	(Hancock+Weistrop+Nelson+, 2006) (Not yet in Simbad)
Write:	<<[HWN2006] NN>>
N:	14
Object:	Region (SIMBAD class: Region = Region defined in the Sky)
Note:	Space Telescope Imaging Spectrograph observations of NGC 4194: 14 star-forming regions (knots) are presented.
in source:	NGC 4194
Ref:	=2006AJ....131..282H
by	HANCOCK M. , WEISTROP D., NELSON C.H., KAISER M.E.
	Astron. J., 131, 282-295 (2006)
	A spectroscopic study of the star-forming properties of the center of NGC 4194.
o	Erratum vol.132, p. 969 (2006)
o	Table 2: <[HWN2006] NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HWS2003]
[HWS2003]	(Hunsch+Weidner+Schmitt, 2003)
Write:	<<[HWS2003] XNNN>>
N:	188
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT X-ray observations and UBVR photometry with the ESO 0.9m Dutch telescope of NGC 2451.
in source:	NGC 2451
Ref:	=2003A&A...402..571H
by	HUENSCH M. , WEIDNER C., SCHMITT J.H.M.M.
	Astron. Astrophys., 402, 571-586 (2003)
	An X-ray study of the open clusters NGC 2451 A and B.
o	Tables 3-10: <[HWS2003] XNNN> (Nos X1-X188).
=E=	Catalogue in electronic form as J/A+A/402/571
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HWW
HWW	(Harju+Walmsley+Wouterlout)
Write:	<<HWW HHMMm+DDMMa>>
N:	27+26+6
Object:	Clump (SIMBAD class: Radio = Radio Source)
Note:	Study of NH3 cores (or clumps) in IRAS in Orion, Cepheus, and some other clouds. HHMMm+DDMMa objects are associated to an IRAS source, HHMMm+DDMMb, c, d are additional clumps. Maps.
Ref:	=1993A&AS...98...51H
by	HARJU J. , WALMSLEY C.M., WOUTERLOOT J.G.A.
	Astron. Astrophys., Suppl. Ser., 98, 51-76 (1993)
	Ammonia clumps in the Orion and Cepheus clouds.
o	Tables 1, 2, 3: <HWW HHMMm+DDMMa> N=26+26+6.
Ref:	=1999ApJ...512..724B
by	BERGIN E.A. , PLUME R., WILLIAMS J.P., MYERS P.C.
	Astrophys. J., 512, 724-739 (1999)
	The ionization fraction in dense molecular gas. II. Massive cores.
o	Table 3: <HWW 05389-0756d> N=1 added.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HWZ2019]
[HWZ2019]	(Hu+Wang+Zheng+, 2019) (Not yet in Simbad)
Write:	<<[HWZ2019] COSMOS-NN>> <<[HWZ2019] CDFS-NN>>
N:	49+30
Object:	LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	CTIO DECam observations of N=49+30 LAEs at z∼7 in the COSMOS and CDFS fields, as part of the Lyman Alpha Galaxies in the Epoch of Reionization (LAGER) project. See also [ZWR2017], [YIR2019], [HWI2021], [HWM2022].
in source:	NAME COSMOS Field
in source:	NAME CDFS Field
Ref:	=2019ApJ...886...90H
by	HU W. , WANG J., ZHENG Z.-Y., MALHOTRA S., RHOADS J.E., INFANTE L., BARRIENTOS L.F., YANG H., JIANG C., KANG W., PEREZ L.A., WOLD I., HIBON P., JIANG L., KHOSTOVAN A.A., VALDES F., WALKER A.R., GALAZ G., COUGHLIN A., HARISH S., KONG X., PHARO J., ZHENG X.
	Astrophys. J., 886, 90-90 (2019)
	The Lyα luminosity function and cosmic Reionization at z ~ 7.0: a tale of two LAGER fields.
o	Fig. 11: <[HWZ2019] COSMOS-NN> (Nos 1-49), <[HWZ2019] CDFS-NN> (Nos 1-30).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: HX
HX	(Hard X)
*****	Avoid the usage of HX, prefer [KLS2002]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HXH2021]
[HXH2021]	(He+Xu+Hao+, 2021)
Write:	<<[HXH2021] NN>>
N:	74
Object:	Poss. Open Cluster of * (SIMBAD class: Cluster*_Candidate = Cluster of Stars Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=74 open cluster candidates within \|b\|<20°. Use of Gaia DR2 data. See also [HXW2020].
Ref:	=2021RAA....21...93H
by	HE Z.-H. , XU Y., HAO C.-J., WU Z.-Y., LI J.-J.
	RAA, 21, 93-93 (2021)
	A catalogue of 74 new open clusters found in Gaia Data-Release 2.
o	Table 1: <[HXH2021] NN> (Nos 1-74).
=E=	Catalogue in electronic form as <J/other/RAA/21.93/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HXW2020]
[HXW2020]	(Hao+Xu+Wu+, 2020)
Write:	<<[HXW2020] OC-NN>>
N:	16
Object:	Poss. Open Cluster of * (SIMBAD class: Cluster*_Candidate = Cluster of Stars Candidate)
Note:	N=16 open cluster (OC) candidates, using Gaia DR2 data. See also [HXH2021].
Ref:	=2020PASP..132c4502H
by	HAO C. , XU Y., WU Z., HE Z., BIAN S.
	PASP, 132c, 4502-34502 (2020)
	Sixteen open clusters discovered with sample-based clustering search of Gaia DR2.
o	(Erratum) erratum vol. 133, id. 059201 (e9201)
o	Table 2: <[HXW2020] OC-NN> (Nos 1-16).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HXX2004]
[HXX2004]	(Huo+Xue+Xu+, 2004)
Write:	<<[HXX2004] A>> <<[HXX2004] WW Clump>>
N:	5+2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	CXO and Keck telescope observations of ClG J0152-1357. 5 point-like sources and 2 diffuse peaks of diffuse emission are found.
in source:	ClG J0152-1357 = RX J0152.7-1357
Ref:	=2004AJ....127.1263H
by	HUO Z.-Y. , XUE S.-J., XU H., SQUIRES G., ROSATI P.
	Astron. J., 127, 1263-1273 (2004)
	Joint X-ray and optical measurements of the mass distribution of the distant galaxy cluster Cl J0152.7-1357.
o	Fig.2, Table 2: <[HXX2004] A> (Nos A-E). Text: <[HXX2004] WW Clump> (Nos NE, SW).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HYC2016]
[HYC2016]	(Harrington+Yun+Cybulski+, 2016)
Write:	<<[HYC2016] PJHHMMSS.s>>
N:	8
Object:	smm G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	LMT AzTEC and RSR 1.1m continuum imaging and CO spectroscopy of N=8 extremely bright submillimetre galaxies identified from the Planck and Herschel surveys.
Ref:	=2016MNRAS.458.4383H
by	HARRINGTON K.C. , YUN M.S., CYBULSKI R., WILSON G.W., ARETXAGA I., CHAVEZ M., DE LA LUZ V., ERICKSON N., FERRUSCA D., GALLUP A.D., HUGHES D.H., MONTANA A., NARAYANAN G., SANCHEZ-ARGUELLES D., SCHLOERB F.P., SOUCCAR K., TERLEVICH E., TERLEVICH R., ZEBALLOS M., ZAVALA J.A.
	Mon. Not. R. Astron. Soc., 458, 4383-4399 (2016)
	Early science with the Large Millimeter Telescope: observations of extremely luminous high-z sources identified by Planck.
o	Figs 6-7, Tables 1-5: <[HYC2016] PJHHMMSS.s> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Hyn
Hyn	(Hynek)
Write:	<<Hyn NNN>>
Object:	* (SIMBAD class: Star)
Note:	Yerkes spectrograph observations.
Ref:	=1938CoPer...1...10H
by	HYNEK J.A.
	Ohio State and Wesleyan Universities - Contributions from the Perkins Observatory, Delaware, Ohio, 1, 10-None (1938)
	A survey of stars with composite spectra.
o	Tables 1, 2: <Hyn NNN> (Nos 1-566).
Origin	of the Acronym: L (2007AN....328...46C)
Details on Acronym: Hyp
Hyp	(Hypergalaxy)
Write:	<<Hyp NN>>
N:	60
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Ref:	=1977TarOT..49....3E
by	EINASTO J. , JOEVEER M., KAASIK A., KALAMEES P., VENNIK J.
	Tartu Astrof. Obs. Teated, 49, 3-73 (1977)
	A list of Hypergalaxies.
o	Table 1: <Hyp NN> (Nos 1-60)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: HZ
HZ	(Humason+Zwicky)= (H-Z)
Write:	<<HZ NNA>>
N:	48
Object:	Blue * (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	(Nos 1-15) are in the region of Hyades, and are also designated as Cl* Melotte 25 HZ in the SIMBAD database. (Nos 16-48) are near the Northern Galactic Pole. No. 43 = No.43A has a faint companion found as '43B' in literature.
in source:	NAME Hyades
in source:	NAME NGP
Ref:	=1947ApJ...105...85H
by	HUMASON M.L. , ZWICKY F.
	Astrophys. J., 105, 85-91 (1947)
	A search for faint blue stars.
o	Table 1: <HZ NN> (Nos 1-48) = <Cl* Melotte 25 HZ NN> for (Nos 1-15).
=E=	Catalogue in electronic form as <J/ApJ/105/85/>
Details on Acronym: Hz
Hz	(Herzog)
Write:	<<NAME Hz II N>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Note:	Herzog E., 1963, Palomar Sky Survey. One object is found in the literature, first in ref. 1976ApJ...209..382L: 'II Hz 4' is the 4th entry in an informal second list of peculiar galaxies compiled by Herzog, so Arp, in 1965, designated this galaxy as 'II Hz 4', NAME II Hz 4 in SIMBAD.
Auth.:	HERZOG E.
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [HZ2006a]
[HZ2006a]	(Hill+Zaritsky, 2006)
*****	Avoid the usage of [HZ2006a], prefer [RZ2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HZ2006b]
[HZ2006b]	(Harris+Zaritsky, 2006)
Write:	<<[HZ2006b] sNN-NNNN>>
N:	2046
Object:	* (SIMBAD class: Star)
Note:	Spectroscopic observations at the Magellan Baade telescope. Survey of 2046 red giant stars in the SMC.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2006AJ....131.2514H
by	HARRIS J. , ZARITSKY D.
	Astron. J., 131, 2514-2524 (2006)
	Spectroscopic survey of red giants in the Small Magellanic Cloud. I. Kinematics.
o	Table 2: <[HZ2006b] sNN-NNNNN> N=2046.
=E=	Catalogue in electronic form as J/AJ/131/2514
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HZK2007]
[HZK2007]	(Hempel+Zepf+Kundu+, 2007)
Write:	<<[HZK2007] NGC4472 NN>> <<[HZK2007] NGC4594 NN>> <<[HZK2007] NGC3585 NN>> <<[HZK2007] NGC5813 NN>>
N:	37+26+26+22
Object:	GlC (SIMBAD class: GlobCluster = Globular Cluster)
Note:	Las Campanas Magellan 6.5m telescope near-infrared photometry of N=37+26+26+22 globular cluster system of the early-type galaxies NGC 4472,NGC 4594, NGC 3585, and NGC 5813. Use of archival HSTand FORS/VLT data.
in source:	NGC 4472
in source:	NGC 4594
in source:	NGC 3585
in source:	NGC 5813
Ref:	=2007ApJ...661..768H
by	HEMPEL M. , ZEPF S., KUNDU A., GEISLER D., MACCARONE T.J.
	Astrophys. J., 661, 768-778 (2007)
	Near-infrared observations of globular clusters in NGC 4472, NGC 4594, NGC 3585, and NGC 5813 and implications for their ages and metallicities.
o	Table 4: <[HZK2007] NGC 4472 NN> (Nos 1-37), Table 5: <[HZK2007] NGC4594 NN> (Nos 1-26), Table 6 <[HZK2007] NGC3585 NN> (Nos 1-26), Table 7: <[HZK2007] NGC5813 NN> (Nos 1-22).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HZR2011]
[HZR2011]	(Huang+Zheng+Rigopoulou+, 2011)= (ERS)
Write:	<<[HZR2011] ERS-N>>
N:	4
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC3 YJH band and Spitzer IRAC observations of the GOODS-South field to search for Extremely Red Sources.
in source:	NAME GOODS South Field
Ref:	=2011ApJ...742L..13H
by	HUANG J.-S. , ZHENG X.Z., RIGOPOULOU D., MAGDIS G., FAZIO G.G., WANG T.
	Astrophys. J., 742L, 13 (2011)
	Four IRAC sources with an extremely red H - [3.6] color: passive or dusty galaxies at z > 4.5?
o	Fig. 1, Table 1: <[HZR2011] ERS-N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: HzRG
HzRG	(High redshift Radio Galaxy)
*****	Avoid the usage of HzRG, prefer [IDS2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [HZS2004]
[HZS2004]	(Hunter+Zhang+Sridharan, 2004) (Not yet in Simbad)
Write:	<<[HZS2004] C18O NN>> <<[HZS2004] Star NNN>>
N:	26+44
Object:	Clump + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Images of the massive star forming region IRAS 18317-0757. N=18 C18O clumps are found. In the 2MASS All Sky Data Release Point Source catalog there are 123 objects within 1' radius of IRAS 18317-0757, and 44 of these stars are in Table 7. See also [HCW2000].
in source:	IRAS 18317-0757
Ref:	=2004ApJ...606..929H
by	HUNTER T.R. , ZHANG Q., SRIDHARAN T.K.
	Astrophys. J., 606, 929-942 (2004)
	IRAS 18317-0757: a cluster of embedded massive stars and protostars.
o	Table 1, Fig.2: <[HCW2000] IRAS 18317-0757 SMM N> (Nos 3-5) added. Table 5: <[HZS2004] C18O NN> (Nos 1-26). Table 7: <[HZS2004] Star NNN> N=44 among 123.
=E=	Catalogue in electronic form as J/ApJ/606/929
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HZV99]
[HZV99]	(Hough+Zensus+Vermeulen+, 1999) (Not yet in Simbad)
Write:	<<[HZV99] 3C NNN C>> <<[HZV99] 3C NNN JN>> <<[HZV99] HHMM+DDd C>> <<[HZV99] HHMM+DDd JN>>
N:	18
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	N=18 components of 7 QSO In the format, the letter 'C' stands for Center, 'JN' for Jet components.
in source:	3C 175
in source:	3C 204
in source:	3C 205
in source:	3C 215
in source:	3C 351
in source:	QSO B0821+447
in source:	QSO B0839+616
Ref:	=1999ApJ...511...84H
by	HOUGH D.H. , ZENSUS J.A., VERMEULEN R.C., READHEAD A.C.S., PORCAS R.W., RIUS A., RECTOR T.A., LENZ G.C., DAVIS M.A., SNOWDALL J.C.
	Astrophys. J., 511, 84-104 (1999)
	Deep 8.4 GHz VLBI images of seven faint nuclei in lobe-dominated quasars.
o	Table 2: <[HZV99] 3C NNN C>, <[HZV99] 3C NNN JN>, <[HZV99] HHMM+DDd C>, <[HZV99] HHMM+DDd JN>, N=18.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [HZW2015]
[HZW2015]	(Huang+Zheng+Wang+, 2015)
Write:	<<[HZW2015] ANN>>
N:	40+12
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	HST ACS WFC and WFC3 (IR and UVIS) observations of N=40+12 extreme emission-line galaxies (EELGs) in 25 CLASH cluster fields.
Ref:	=2015ApJ...801...12H
by	HUANG X. , ZHENG W., WANG J., FORD H., LEMZE D., MOUSTAKAS J., SHU X., VAN DER WEL A., ZITRIN A., FRYE B.L., POSTMAN M., BARTELMANN M., BENITEZ N., BRADLEY L., BROADHURST T., COE D., DONAHUE M., INFANTE L., KELSON D., KOEKEMOER A., LAHAV O., MEDEZINSKI E., MOUSTAKAS L., ROSATI P., SEITZ S., UMETSU K.
	Astrophys. J., 801, 12 (2015)
	CLASH: extreme emission-line galaxies and their implication on selection of high-redshift galaxies.
o	Table 1: <[HZW2015] JNN (Nos 1-40), Table 2: <[HZW2015] YNN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: I
I	(Intermediate source) (Not yet in Simbad)
Write:	<<I HHMM+DD>> <<I HHMM+DDd>>
N:	72
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Table III
Ref:	=1972AJ.....77..265P
by	PAULINY-TOTH I.I.K. , KELLERMANN K.I., DAVIS M.M., FOMALONT E.B., SHAFFER D.B.
	Astron. J., 77, 265-284 (1972)
	The NRAO 5-GHz radio source survey. II. The 140-ft "Strong", "Intermediate", and "Deep" source surveys.
o	Table II: <S1 HHMM+DD> N=27, <S2 HHMM+DD>, <S2 HHMM+DDd> N=218. Table III: <I HHMM+DD>, <I HHMM+DDd> N=72
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: I
I	(IRAC)
*****	Avoid the usage of I, prefer [GHB2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: I
I	(Ichikawa)
*****	Avoid the usage of I, prefer [I81]
Origin	of the Acronym: L (1987AnTok..21..293M)
Details on Acronym: I
I	(Ivanov)
*****	Avoid the usage of I, prefer [I85]
Origin	of the Acronym: L (1996IBVS.4411....1N)
Details on Acronym: I
I	(Roman num. list I)
*****	Avoid the usage of I, prefer IC
Details on Acronym: I
I	(Ichikawa)
*****	Avoid the usage of I, prefer Kiso
Origin	of the Acronym: L = Found in the literature
Details on Acronym: I2000
I2000	(Imai+, 2000) (Not yet in Simbad)
*****	Avoid the usage of I2000, prefer [IKS2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [I2002]
[I2002]	(Ivanov, 2002)= ([I2002a])
Write:	<<[I2002] JHHMMSS.ss+DDMMSS.s>>
N:	2
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	FORS1 VLT observations. Search for the optical counterpart of the X-ray jet candidate CXOU J130609.3+035643 near SDSS J130608.26+035626.3. 2 candidates are found.
Ref:	=2002A&A...389L..37I
by	IVANOV V.D.
	Astron. Astrophys., 389, 37-38 (2002)
	Deep I-band imaging of z=5.99 quasar.
o	Schwartz paper cited as astro-ph/0202190 was published as 2002ApJ...571L..71S.
o	Text: <[I2002] JHHMMSS.ss+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [I2002a]
[I2002a]	(Ivanov, 2002)
*****	Avoid the usage of [I2002a], prefer [I2002]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [I2002b]
[I2002b]	(Iovino, 2002) (Not yet in Simbad)
Write:	<<[I2002b] HHMM+DDMM A>>
N:	519
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Note:	Galaxies from the brightest (No. A) to fainter members in SCG2 groups.
Ref:	=2002AJ....124.2471I
by	IOVINO A.
	Astron. J., 124, 2471-2489 (2002)
	Detecting fainter compact groups: results from a new automated algorithm.
o	Table 1: <SCG2 HHMM+DDMM> N=121. Figs 3: <[I2002b] HHMM+DDMM A> N=519.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: I2007
I2007	(Imai, 2007) (Not yet in Simbad)
Write:	<<I2007 IRAS 19134+2131 NN>>
N:	20
Object:	H2O Maser (SIMBAD class: Maser)
Note:	Use of the Very Long Baseline Array to study H2O maser emission in IRAS 19134+2131. The numbering 'NN' stands for the sources found by Imai+ in 2007, IAU Symp. 242, Astrophysical Masers and their Environments.
in source:	IRAS 19134+2131
Ref:	=2007ApJ...669..424I
by	IMAI H. , SAHAI R., MORRIS M.
	Astrophys. J., 669, 424-434 (2007)
	The spatio-kinematical structure and distance of the preplanetary nebula IRAS 19134+2131.
o	Table 3: <I2007 IRAS 19134+2131 NN> (Nos 1-20).
=E=	Catalogue in electronic form as J/ApJ/669/424
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [I2022]
[I2022]	(Ibarra-Medel, 2022)
Write:	<<[I2022] A>> <<[I2022] J004150-091812>>
N:	14+1
Object:	G + QSO + * + Poss. Group of G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=14 sources and N=1 compact galaxy group candidate behind [H37] 15a. Use of MUSE archival data.
in source:	[H37] 15a = MCG-02-02-086
Ref:	=2022MNRAS.515.6032I
by	IBARRA-MEDEL H.
	Mon. Not. R. Astron. Soc., 515, 6032-6045 (2022)
	A spectroscopic study of 14 structures behind Holm15A: detecting a galaxy group candidate at z = 0.58.
o	Fig. 1, Table 1: <[I2022] A> (Nos A-O). Text: <[I2022] J004150-091812> N=1.
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [I59]
[I59]	(Ikhsanov, 1959)= (Ih)
Write:	<<[I59] +DD NNN>>
N:	952
Object:	* (SIMBAD class: Star)
Note:	* in the zones +39deg to +44deg
Ref:	=1959IzKry..21..229I
by	IKHSANOV N.R.
	Izv. Krym. Astrofiz. Obs., 21, 229-256 (1959)
	The spectra, magnitudes and colours of O-A type stars in an area of the Milky Way, with the Center α = 20h16m, δ = +42 D 30'.
o	<[I59] +39 NNN> (Nos 1-136), <[I59] +40 NNN> (Nos 1-209), <[I59] +41 NNN> (Nos 1-204), <[I59] +42 NNN> (Nos 1-191), <[I59] +43 NNN> (Nos 1-138), <[I59] +44 NN> (Nos 1-74)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [I60]
[I60]	(Ikhsanov, 1960)
Write:	<<[I60] IC 1318a>>
N:	3
Object:	Nebula (SIMBAD class: ISM = Interstellar Medium Object)
Note:	N=3 bright emission regions or nebulae in IC 1318.
in source:	IC 1318
Ref:	=1960SvA.....4..258I
by	IKHSANOV R.N.
	Sov. Astron., 4, 258-263 (1960)
	Nebulae 1318a, 1318b, 1318c, and interstellar absorption.
o	<[I60] IC 1318a> (Nos a-c).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [I68]
[I68]	(Isserstedt, 1968)= (SR) (Not yet in Simbad)
Write:	<<[I68] NNNN>> <<[I68] Anon NNa>>
N:	1002+89
Object:	* Ring (SIMBAD class: Star)
Ref:	=1968VeBoc...1....1I
by	ISSERSTEDT J.
	Veroeff. Astron. Inst. Ruhr-Univ. Bochum, 1, 1-79 (1968)
	Sternringe, eine neue art von sternaggregaten und ihre beziehung zur galaktischen struktur.
o	<[I68] NNNN> (Nos 1-1002)
Ref:	=1973ACiCh.772....4U
by	URANOVA T.A.
	Astron. Cir., 772, 4-6 (1973)
	Supplement list of stellar rings. I.
o	Table: <[I68] Anon NNa> (Nos 1-20, 21a-21b, 22-46)
Ref:	=1973ACiCh.773....3U
by	URANOVA T.A.
	Astron. Cir., 773, 3-5 (1973)
	Supplement list of stellar rings. II.
o	Table: <[I68] Anon NN> (Nos 47-88)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [I75]
[I75]	(Israel, 1975) (Not yet in Simbad)
Write:	<<[I75] NN>>
N:	39
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Map in Fig.1b. N=39 sources outside the optical image of M 101 except Nos 20 and 22.
in source:	M 101 = NGC 5457
Ref:	=1975A&A....40..421I
by	ISRAEL F.P. , GOSS W.M., ALLEN R.J.
	Astron. Astrophys., 40, 421-438 (1975)
	The giant spiral galaxy M 101: radio observations of H II regions in external galaxies.
o	Table 1: <NAME GOSS I>. Table 5: <[I75] NN> (Nos 1-39)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [I77]
[I77]	(Israel, 1977)
Write:	<<[I77] DR 15 A>> <<[I77] S 184 A>> <<[I77] S 228 A>> <<[I77] NN>>
N:	6+2+2+44
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Radio-components of HII regions: DR 15: (Nos A-I). Sh 2-184: (Nos A-B). Sh 2-228: (Nos C, E) for Core and Envelope. Radio-sources in the fields of 5 HII regions: (Nos 1-44).
Ref:	=1977A&A....60..233I
by	ISRAEL F.P.
	Astron. Astrophys., 60, 233-249 (1977)
	Aperture synthesis observations of galactic H II regions. VI. Several isolated H II regions.
o	Table 7, Figs 9, 16: <[I77] DR 15 A> (Nos A-I), <[I77] S 184 A> (Nos A-B), <[I77] S 228 A> (Nos C, E). Table 8: <[I77] NN> (Nos 1-44).
Ref:	=1980MNRAS.192..377C
by	COLLEY D.
	Mon. Not. R. Astron. Soc., 192, 377-388 (1980)
	Radio observations of DR 15 at 408, 1407 and 2695 MHz.
o	Figs 1, 2, Table 3: <[I77] DR 15 A> (Nos G-I) added. Fig. 2: <[C80b] Star NN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [I80]
[I80]	(Israel, 1980)
Write:	<<[I80] SMC-NN>> <<[I80] LMC-NN>> <<[I80] IC 342-NN>> <<[I80] NGC NNNN-NN>>
N:	19+41+11+102
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Radio observations of 12 galaxies to search for HII regions in each of these galaxies.
Ref:	=1980A&A....90..246I
by	ISRAEL F.P.
	Astron. Astrophys., 90, 246-268 (1980)
	Radio observations of H II regions in external galaxies. III - Thermal emission, H II regions and star formation in 14 late-type galaxies.
o	Table 2a: <[I80] SMC-NN> (Nos 1-18), <[I80] LMC-NN> (Nos 1-41). Table 2b: <[I80] IC 342-NN> (Nos 1-11), <[I80] NGC NNNN-NN> N=102.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [I81]
[I81]	(Ichikawa, 1981)= (I)
Write:	<<[I81] M NNN>> <<[I81] C MM>> <<[I81] S N>>
N:	722+34+2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 2: 'M' in the format stands for 'M ', (Nos 1-722). Table 3: 'C' in the format stands for 'Carbon ', (Nos 1-34). Table 4: 'S' in the format stands for 'S *', (Nos 1-2)
Ref:	=1981PASJ...33..107I
by	ICHIKAWA T.
	Publ. Astron. Soc. Jap., 33, 107-133 (1981)
	The space distribution of M giants in the direction of Cas.
o	Wrong positions for [I81] M 352, 430, 471, 566 and 301 ; corrected in SIMBAD by B. Skiff (August 30, 2004)
o	Table 2: <[I81] M NNN> (Nos 1-722). Table 3: <[I81] C NN> (Nos 1-34). Table 4: <[I81] S N> (Nos 1-2).
=E=	Catalogue in electronic form as J/other/PASJ/33.107
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [I82]
[I82]	(Irvine, 1982)
Write:	<<[I82] Globule N>> <<[I82] Em* N>>
N:	8+3
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=8 nebular features or globules and N=3 faint emission stars in the vicinity of * alf Mus.
Ref:	=1982PASP...94..239I
by	IRVINE N.J.
	Publ. Astron. Soc. Pac., 94, 239-243 (1982)
	Emission globules in Musca.
o	Fig.1, Table I: <[I82] Globule N> (Nos 1-8). Fig.2, Table II: <[I82] Em* N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [I85]
[I85]	(Ivanov, 1985)= (I)
Write:	<<[I85] V1>> <<[I85] N>>
N:	1+7
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=1 new variable star is found in M 31, called 'V' by the authors, 'V1' by SIMBAD. N=7 companion stars
in source:	M 31 = NGC 224
Ref:	=1985Ap&SS.115..409I
by	IVANOV G.R.
	Astrophys. Space Sci., 115, 409-411 (1985)
	A new 75-day Cepheid in M 31.
o	<[I85] V1> N=1, <[I85] N> (Nos 1-7)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [I91]
[I91]	(Ibragimov, 1991)
Note:	The same paper has been published in 1993AZh....70..339I,
*****	Avoid the usage of [I91], prefer [I93]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [I92a]
[I92a]	(Ivanov, 1992)
Write:	<<[I92a] NNN>>
N:	185
Object:	Non-stellar Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
in source:	M 33 = NGC 598
Ref:	=1992ApL....28..281I
by	IVANOV G.R.
	Astrophys. Lett., 28, 281-289 (1992)
	Nonstellar objects in M 33.
o	<[I92a] NNN> N=185
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [I92b]
[I92b]	(Ivanov, 1992)
Write:	<<[I92b] NNN>>
N:	180
Object:	OB Assoc. (SIMBAD class: Association = Association of Stars)
Stat:	is completely incorporated in Simbad
in source:	M 81 = NGC 3031
Ref:	=1992MNRAS.257..119I
by	IVANOV G.R.
	Mon. Not. R. Astron. Soc., 257, 119-124 (1992)
	Stellar associations in M 81.
o	Table 1: <[I92b] NNN> N=180.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [I93]
[I93]	(Ibragimov, 1993)= ([I91])
Write:	<<[I93] NN>> <<[I93] MNN>>
N:	65+10
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Format 'MNN': * projected onto B35. The same paper has first been published in 1991Afz....35...11I
Ref:	=1993AZh....70..339I
by	IBRAGIMOV M.A.
	Astron. Zh., 70, 339-349 (1993)
	Observational study of Fuors. FU Orionis in 1984-1990. A remarkable change in the brightness decline rate.
o	Same paper in 1991Afz....35...11I
o	Table 4: <[I93] NN> (Nos 1-65), <[I93] MNN> (Nos M1-M10)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: I96
I96	(Israel+, 1996)
*****	Avoid the usage of I96, prefer [IBK96]
Origin	of the Acronym: L (2006ApJ...652.1170C)
Details on Acronym: [IAB2009]
[IAB2009]	(Irwin+Aigrain+Bouvier+, 2009)
Write:	<<[IAB2009] M50-N-NNNN>>
N:	812
Object:	* (SIMBAD class: Star)
Note:	CTIO 4m Blanco telescope photometry of low-mass stars in M50.
in source:	M 50 = NGC 2323
Ref:	=2009MNRAS.392.1456I
by	IRWIN J. , AIGRAIN S., BOUVIER J., HEBB L., HODGKIN S., IRWIN M., MORAUX E.
	Mon. Not. R. Astron. Soc., 392, 1456-1466 (2009)
	The monitor project: rotation periods of low-mass stars in M50.
o	Table 1: <[IAB2009] M50-N-NNNN> N=812 among (Nos 98-1130).
=E=	Catalogue in electronic form as J/MNRAS/392/1456
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IAC
IAC	(Instituto de Astrofisica de Canarias)
Write:	<<IAC JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	Grav. lens system
Stat:	is completely incorporated in Simbad
Note:	We propose the registration of a single object after the publication of the discovery paper entitled "The Canarias Einstein Ring: a Newly Discovered Optical Einstein Ring" on the peer review scientific journal MNRAS Letters. Here below the link to the publication. http://mnrasl.oxfordjournals.org/content/461/1/L67
Ref:	=2016MNRAS.461L..67B
by	BETTINELLI M. , SIMIONI M., APARICIO A., HIDALGO S.L., CASSISI S., WALKER A.R., PIOTTO G., VALDES F.
	Mon. Not. R. Astron. Soc., 461L, 67-71 (2016)
	The Canarias Einstein ring: a newly discovered optical Einstein ring.
o	<IAC J010127.83-334319.6> N=1 = <NAME Canarias Einstein ring> N=1. <[BSA2016] lens> N=1. <[BSA2016] source> N=1.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: IAU
IAU	(International Astronomical Union) (Not yet in Simbad)
*****	Avoid the usage of IAU, prefer [P55]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: Iban
Iban	(Ibanez)
Write:	<<IBAN NN>>
N:	13
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Ref:	=1977IBVS.1246....1I
by	IBANEZ M.
	IAU Inform. Bull. Var. Stars, 1246, 1-3 (1977)
	Radial velocities of Me type stars.
o	IBAN
o	Table: <IBAN NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IBB2003]
[IBB2003]	(Inada+Becker+Burles+, 2003)
Write:	<<[IBB2003] SDSS J0924+0219>> <<[IBB2003] SDSS J0924+0219 A>> <<[IBB2003] SDSS J0924+0219 A'>> <<[IBB2003] Star a>>
N:	1+5+1+5
Object:	Grav. lens system + Grav. lens + Grav. lensed image + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	SDSS and follow-up WB Las Campanas and Keck II observations. SDSS J092455.87+021924.9 is a lensed QSO with lensed images (Nos A-D) and an other predicted image D', a lensing galaxy G. In the field of the QSO, 3 stars then 2 more are identified.
Ref:	=2003AJ....126..666I
by	INADA N. , BECKER R.H., BURLES S., CASTANDER F.J., EISENSTEIN D., HALL P.B., JOHNSTON D.E., PINDOR B., RICHARDS G.T., SCHECHTER P.L., SEKIGUCHI M., WHITE R.L., BRINKMANN J., FRIEMAN J.A., KLEINMAN S.J., KRZESINSKI J., LONG D.C., NEILSEN E.H.Jr, NEWMAN P.R., NITTA A., SCHNEIDER D.P., SNEDDEN S., YORK D.G.
	Astron. J., 126, 666-674 (2003)
	SDSS J092455.87+021924.9: an interesting gravitationally lensed quasar from the Sloan Digital Sky Survey.
o	Text: <[IBB2003] SDSS J0924+0219> N=1. Tables 2, 4: <[IBB2003] SDSS J0924+0219 A> (Nos A-D, G), <[IBB2003] SDSS J0924+0219 A'> (No. D'), <[IBB2003] Star a> (Nos a-c).
Ref:	=2006A&A...451..747E
by	EIGENBROD A. , COURBIN F., DYE S., MEYLAN G., SLUSE D., VUISSOZ C., MAGAIN P.
	Astron. Astrophys., 451, 747-757 (2006)
	COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses. II. SDSS J0924+0219: the redshift of the lensing galaxy, the quasar spectral variability and the Einstein rings.
o	Fig.1: <[IBB2003] Star a> (Nos d-e) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IBB2011]
[IBB2011]	(Imara+Bigiel+Blitz, 2011)
Write:	<<[IBB2011] NNA>>
N:	45
Object:	HI (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 21cm observations of HI clumps which do not contain giant molecular clouds.
in source:	M 33 = NGC 598
Ref:	=2011ApJ...732...79I
by	IMARA N. , BIGIEL F., BLITZ L.
	Astrophys. J., 732, 79 (2011)
	Angular momentum in giant molecular clouds. II. M33.
o	Table 2: <[IBB2011] NNA> (Nos 1A-45A).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IBB2017]
[IBB2017]	(Inami+Bacon+Brinchmann+, 2017)= (MUSE)
Write:	<<[IBB2017] NNNN>>
N:	1574+2221
Object:	G (SIMBAD class: Galaxy)
Note:	VLT MUSE (Multi Unit Spectroscopic Explorer) observations of N=1574+2221 galaxies as part of the MUSE Hubble Ultra Deep Field survey (number of sources in DR1 and DR2 respectively).
Ref:	=2017A&A...608A...2I
by	INAMI H. , BACON R., BRINCHMANN J., RICHARD J., CONTINI T., CONSEIL S., HAMER S., AKHLAGHI M., BOUCHE N., CLEMENT B., DESPREZ G., DRAKE A.B., HASHIMOTO T., LECLERCQ F., MASEDA M., MICHEL-DANSAC L., PAALVAST M., TRESSE L., VENTOU E., KOLLATSCHNY W., BOOGAARD L.A., FINLEY H., MARINO R.A., SCHAYE J., WISOTZKI L.
	Astron. Astrophys., 608A, 2-2 (2017)
	The MUSE Hubble Ultra Deep Field Survey. II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxies.
o	udf-10, mosaic, combined: <[IBB2017] NNNN> N=313+1439+1574 among (Nos 1-7582).
Ref:	=2023A&A...670A...4B
by	BACON R. , BRINCHMANN J., CONSEIL S., MASEDA M., NANAYAKKARA T., WENDT M., BACHER R., MARY D., WEILBACHER P.M., KRAJNOVIC D., BOOGAARD L., BOUCHE N., CONTINI T., EPINAT B., FELTRE A., GUO Y., HERENZ C., KOLLATSCHNY W., KUSAKABE H., LECLERCQ F., MICHEL-DANSAC L., PELLO R., RICHARD J., ROTH M., SALVIGNOL G., SCHAYE J., STEINMETZ M., TRESSE L., URRUTIA T., VERHAMME A., VITTE E., WISOTZKI L., ZOUTENDIJK S.L.
	Astron. Astrophys., 670A, 4 (2023)
	The MUSE Hubble Ultra Deep Field surveys: Data release II.
o	<[IBB2017] NNNN> N=2221 among (Nos 1-8591).
=E=	Catalogue in electronic form as <J/A+A/608/A2/>
=E=	Catalogue in electronic form as <J/A+A/670/A4/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [IBB2020]
[IBB2020]	(Ivison+Biggs+Bremer+, 2020)
Write:	<<[IBB2020] JHHMMSS.ss+DDMMSS.s>> <<[IBB2020] DRC-D'>>
N:	5+1
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	ALMA Band 3 observations of N=5+1 sources in the field of the Distant Red Core (DRC) at z=4.0.
in source:	[OID2018] DRC cluster
Ref:	=2020MNRAS.496.4358I
by	IVISON R.J. , BIGGS A.D., BREMER M., ARUMUGAM V., DUNNE L.
	Mon. Not. R. Astron. Soc., 496, 4358-4365 (2020)
	ALMA unveils wider environment of distant red protocluster core.
o	Figs 1-2, Table 1: <[IBB2020] JHHMMSS.ss+DDMMSS.s> N=5. Paragr. 3.1: <[IBB2020] DRC-D'> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IBC2002]
[IBC2002]	(Iglesias-Paramo+Boselli+Cortese+, 2002)
Write:	<<[IBC2002] JHHMMSS+DDMMSS>>
N:	41+22
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=41 H-alpha emitting galaxies in ACO 1367. N=22 H-alpha emitting galaxies in Coma Cluster. See also [IBG2003].
in source:	ACO 1367
in source:	Coma Cluster = ACO 1656
Ref:	=2002A&A...384..383I
by	IGLESIAS-PARAMO J. , BOSELLI A., CORTESE L., VILCHEZ J.M., GAVAZZI G.
	Astron. Astrophys., 384, 383-392 (2002)
	A deep Hα survey of galaxies in the two nearby clusters Abell 1367 and Coma. The Hα luminosity functions.
o	Tables 4, 5: <[IBC2002] JHHMMSS+DDMMSS> N=41+22.
=E=	Catalogue in electronic form as J/A+A/384/383
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IBC2013]
[IBC2013]	(Indebetouw+Brogan+Chen+, 2013)
Write:	<<[IBC2013] NNN>> <<[IBC2013] Clump-NNN>> (not recognised by Simbad, but found in literature)
N:	103
Object:	Clump (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	ALMA 12CO(2-1) and 13CO(2-1) observations of N=103 clumps in the 30Dor-10 cloud.
in source:	Magellanic Clouds:LMC:30 Dor Nebula = 30 Dor Nebula
in source:	Magellanic Clouds:LMC:[JGB98] 30 Dor-10 = [JGB98] 30 Dor-10
Ref:	=2013ApJ...774...73I
by	INDEBETOUW R. , BROGAN C., CHEN C.-H.R., LEROY A., JOHNSON K., MULLER E., MADDEN S., CORMIER D., GALLIANO F., HUGHES A., HUNTER T., KAWAMURA A., KEPLEY A., LEBOUTEILLER V., MEIXNER M., OLIVEIRA J.M., ONISHI T., VASYUNINA T.
	Astrophys. J., 774, 73 (2013)
	ALMA resolves 30 Doradus: sub-parsec molecular cloud structure near the closest super star cluster.
o	Table 3: <[IBC2013] NNN> (Nos 1-103).
=E=	Catalogue in electronic form as J/ApJ/774/73
Details on Acronym: [IBG2003]
[IBG2003]	(Iglesias-Paramo+Boselli+Gavazzi+, 2003)
Write:	<<[IBG2003] JHHMMSS+DDMMSS>>
N:	4413+5555
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	WFC INT observations. N=4413 galaxies in ACO 1367 and N=5555 in Coma Cluster. See also [IBG2002], [CGB2004b].
in source:	ACO 1367
in source:	Coma Cluster = ACO 1656
Ref:	=2003A&A...397..421I
by	IGLESIAS-PARAMO J. , BOSELLI A., GAVAZZI G., CORTESE L., VILCHEZ J.M.
	Astron. Astrophys., 397, 421-430 (2003)
	The r'-band luminosity function of Abell 1367: A comparison with Coma.
o	Catalog: <[IBG2003] JHHMMSS+DDMMSS> N=4413+5555.
=E=	Catalogue in electronic form as J/A+A/397/421
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IBG2005]
[IBG2005]	(Inada+Burles+Gregg+, 2005)
Write:	<<[IBG2005] SDSS J0246-0825>> <<[IBG2005] SDSS J0246-0825 A>> <<[IBG2005] SDSS J0246-0825 G'>>
N:	1+3+2
Object:	Grav. lensed image + G (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Stat:	is completely incorporated in Simbad
Note:	Imaging observations with the Keck telescope and the HST. The lensed QSO SDSS J024634.11-082536.2 has 2 images A and B, with a third component C observed as a highly distorded object. Near the primary lensing galaxy G a faint object G' could be a secondary lensing G.
Ref:	=2005AJ....130.1967I
by	INADA N. , BURLES S., GREGG M.D., BECKER R.H., SCHECHTER P.L., EISENSTEIN D.J., OGURI M., CASTANDER F.J., HALL P.B., JOHNSTON D.E., PINDOR B., RICHARDS G.T., SCHNEIDER D.P., WHITE R.L., BRINKMANN J., SZALAY A.S., YORK D.G.
	Astron. J., 130, 1967-1976 (2005)
	SDSS J024634.11-082536.2: a new gravitationally lensed quasar from the Sloan Digital Sky Survey.
o	Fig.2: Star S not identified in SIMBAD.
o	Text: <[IBG2005] SDSS J0246-0825> N=1. Tables 1, 4: <[IBG2005] SDSS J0246-0825 A> (Nos A-C, G), <[IBG2005] SDSS J0246-0825 A'> (No. G').
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IBK96]
[IBK96]	(Israel+Bontekoe+Kester, 1996)= (I96) = (IR)
Write:	<<[IBK96] N>>
N:	9
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	NGC 6822
Ref:	=1996A&A...308..723I
by	ISRAEL F.P. , BONTEKOE T.R., KESTER D.J.M.
	Astron. Astrophys., 308, 723-732 (1996)
	Dust and molecules in the Local Group galaxy NGC 6822. I. Dust, star formation and the origin of infrared emission.
o	H = [H25], Ho = [H77] HII, KD = KD SNN
o	<[IBK96] N> (Nos 1-9)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IBM88]
[IBM88]	(Impey+Bothun+Malin, 1988)
Write:	<<[IBM88] VFFLNN>>
N:	137
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	In the format 'VFFLNN' VFF stands for Virgo fields (Nos V1-V11), No. V5 missing. LNN is a running number in each field.
in source:	NAME Virgo Cluster
Ref:	=1988ApJ...330..634I
by	IMPEY C. , BOTHUN G., MALIN D.
	Astrophys. J., 330, 634-660 (1988)
	Virgo dwarfs : new light on faint galaxies.
o	[IBM88] V11L02 not cross-identified to VCC 1601.
o	<[IBM88] VFFLNN> N=137
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IBP2002]
[IBP2002]	(Ivanov+Borissova+Pessev+, 2002)= (CC) = (Ivanov)
Write:	<<[IBP2002] CCNN>>
N:	14
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Stat:	is completely incorporated in Simbad
Note:	N= 14 Clusters Candidates (CC in the format) in the Milky Way.
Ref:	=2002A&A...394L...1I
by	IVANOV V.D. , BORISSOVA J., PESSEV P., IVANOV G.R., KURTEV R.
	Astron. Astrophys., 394, 1-4 (2002)
	Discovery of new Milky Way star clusters candidates in the 2MASS point source catalog.
o	In reflist, Minkowski : 1948 is a misprint for 1947.
o	Table 1: <[IBP2002] CCNN> (Nos CC01-CC10).
Ref:	=2003A&A...411...83B
by	BORISSOVA J. , PESSEV P., IVANOV V.D., SAVIANE I., KURTEV R., IVANOV G.R.
	Astron. Astrophys., 411, 83-90 (2003)
	Discovery of new Milky Way star cluster candidates in the 2MASS Point Source Catalog. II. Physical properties of the star cluster CC01.
o	IRAS 0553+3421 is a misprint for IRAS 05253+3421. In reflist, Minkowski PASP.59.257 : 1948 is a misprint for 1947.
o	Table 1: <[IBP2002] CCNN> (Nos CC11-CC14) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IBR2011]
[IBR2011]	(Immer+Brunthaler+Reid+, 2011)
Write:	<<[IBR2011] JHHMM+DDMM>>
N:	199+1330
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	VLBA observations of N=199 (detected) + N=1330 (undetected) sources as a preparatory survey for the Bar and Spiral Structure Legacy survey (BeSSeL).
Ref:	=2011ApJS..194...25I
by	IMMER K. , BRUNTHALER A., REID M.J., BARTKIEWICZ A., CHOI Y.K., MENTEN K.M., MOSCADELLI L., SANNA A., WU Y.W., XU Y., ZHANG B., ZHENG X.W.
	Astrophys. J., Suppl. Ser., 194, 25 (2011)
	The VLBA calibrator search for the BeSSeL survey.
o	[IBR2011] J1751-2523 not in SIMBAD.
o	Tables 2-3: <[IBR2011] JHHMM+DDMM> N=199+1330.
=E=	Catalogue in electronic form as <J/ApJS/194/25/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IC
IC	(Imperial College)
*****	Avoid the usage of IC, prefer [GOS97]
Origin	of the Acronym: L (1999A&A...342..313A)
Details on Acronym: IC
IC	(Index Catalog)= (I) or (II) = (IC I) or (IC II)
Write:	<<IC NNNN>>
N:	5386
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	For identifications of NGC and IC numbers in the Magellanic Clouds or in M 33 see Lortet 1986, Astr. Astrophys. Suppl. 64, p. 303-324 for objects in the LMC and SMC, p. 325-328 for objects in M 33. NGC 2000.0: Sinnott, 1988, N=13226 objects (NGC and IC), corrections from several the authors and 700 from Dreyer himself
Ref:	=1895MmRAS..51..185D
by	DREYER J.L.E.
	Mem. R. Astron. Soc., 51, 185-228 (1895)
	Index Catalogue of Nebulae found in the years 1888 to 1894, with Notes and Corrections to the New General Catalogue.
o	Catalogue: <IC NNNN> (Nos 1-1529)
Ref:	=1908MmRAS..59..105D
by	DREYER J.L.E.
	Mem. R. Astron. Soc., 59, 105-198 (1908)
	Index Catalogue of Nebulae and Clusters of Stars, containing objects found in the years 1895 to 1907; with Notes and Corrections to the New General Catalogue and to the Index Catalogue for 1888-94.
o	Catalogue: <IC NNNN> (Nos 1530-5386)
=E=	Catalogue in electronic form as VII/118
Details on Acronym: IC 348-X
IC 348-X	(IC 348, X-ray)
*****	Avoid the usage of IC 348-X, prefer [PZH96]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IC I
IC I	(Index Cat., list I)
*****	Avoid the usage of IC I, prefer IC
Details on Acronym: IC II
IC II	(Index Cat., list II)
*****	Avoid the usage of IC II, prefer IC
Details on Acronym: IC4665
IC4665	(IC 4665)
*****	Avoid the usage of IC4665, prefer [DBP2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [IC54]
[IC54]	(Iriarte+Chavira, 1954) (Not yet in Simbad)
Write:	<<[IC54] NN>>
N:	70
Object:	OB * (SIMBAD class: Star)
Note:	See also [IC55a], [IC55b]. H S
Ref:	=1954BOTT....2j..27I
by	IRIARTE B. , CHAVIRA E.
	Bol. Obs. Tonantz. Tacub., 2, part no 10, 27-33 (1954)
	Nuevas gigantes azules entre longitudes galacticas l = 345 ° a l = 35 °.
o	Tables I and II: numbering 'NN' in first column not used, stars have an HD or BD designations.
o	Table III: <[IC54] NN> (Nos 1-70).
Details on Acronym: [IC55a]
[IC55a]	(Iriarte+Chavira, 1955)
Write:	<<[IC55a] NNN>>
N:	110
Object:	OB * (SIMBAD class: Star)
Note:	See also [IC54], [IC55b].
Ref:	=1955BOTT....2m..12I
by	IRIARTE B. , CHAVIRA E.
	Bol. Obs. Tonantz. Tacub., 2, part no 13, 12-18 (1955)
	Gigantes azules entre l = 330 ° y l = 35 °.
o	Tables I and II: numbering 'NN' in first column not used, stars have an HD or BD designations.
o	Table III: <[IC55a] NNN> (Nos 1-110).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IC55b]
[IC55b]	(Iriarte+Chavira, 1955)
Write:	<<[IC55b] NN>>
N:	79
Object:	OB * (SIMBAD class: EmLine* = Emission-line Star)
Note:	See also [IC54], [IC55a].
Ref:	=1955BOTT....2m..19I
by	IRIARTE B. , CHAVIRA E.
	Bol. Obs. Tonantz. Tacub., 2, part no 13, 19-22 (1955)
	Nuevas estrellas de tipos espectrales tempranos con H α en emision entre l = 338 ° y l = 33 °.
o	Table I: numbering 'NN' in first column not used, stars have a BD designation.
o	Table II: <[IC55b] NN> (Nos 1-79).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IC56]
[IC56]	(Iriarte+Chavira, 1956)= (Ir-Ch)
Write:	<<[IC56] NN>>
N:	55
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Ref:	=1956BOTT....2n..31I
by	IRIARTE B. , CHAVIRA E.
	Bol. Obs. Tonantz. Tacub., 2, part no 14, 31-34 (1956)
	Lista de estrellas con H α en emision entre l = 338 D y l = 33 D.
o	Table I: <[IC56] NN> (Nos 1-55).
Details on Acronym: ICA
ICA	(Inter-Cloud Association)= (BD)
Write:	<<ICA NN>>
N:	78
Object:	Young Assoc. (SIMBAD class: Association = Association of Stars)
Stat:	is completely incorporated in Simbad
in source:	Magellanic Clouds:Magellanic Bridge = Magellanic Bridge
Ref:	=1992AJ....104.1458B
by	BATTINELLI P. , DEMERS S.
	Astron. J., 104, 1458-1464 (1992)
	Automated identification of young associations in the inter-Magellanic Cloud region.
o	Table 1: <ICA NN> N=78
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ICB2018]
[ICB2018]	(Ilee+Cyganowski+Brogan+, 2018)
Write:	<<[ICB2018] G011.92-00.61 MM1a>>
N:	2
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 6 (1.3mm) observations of N=2 sources in the massive young stellar object [CBH2011b] G11.92-0.61 MM1.
in source:	[CBH2011b] G11.92-0.61 MM1
Ref:	=2018ApJ...869L..24I
by	ILEE J.D. , CYGANOWSKI C.J., BROGAN C.L., HUNTER T.R., FORGAN D.H., HAWORTH T.J., CLARKE C.J., HARRIES T.J.
	Astrophys. J., 869L, 24-24 (2018)
	G11.92-0.61 MM 1: a fragmented Keplerian disk surrounding a proto-O star.
o	Fig. 1, Table 1: <[ICB2018] G011.92-00.61 MM1a> (Nos MM1a-MM1b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ICB99]
[ICB99]	(Itoh+Chrysostomou+Burton, 1999)
Write:	<<[ICB99] WN>>
N:	5+5
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=5 H2 emission clumps in the eastern lobe of DR 21. N=5 H2 emission clumps in the western lobe of DR 21. Maps. See also [DS96].
in source:	DR 21
Ref:	=1999MNRAS.304..406I
by	ITOH Y. , CHRYSOSTOMOU A., BURTON M., HOUGH J.H., TAMURA M.
	Mon. Not. R. Astron. Soc., 304, 406-414 (1999)
	The magnetic field structure of the DR 21 region.
o	Fig.1: <[DS96] O3> added. Table 2: <[ICB99] WN> (Nos E1-E5, W1-W5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ICC2000]
[ICC2000]	(Israel+Covino+Campana+, 2000) (Not yet in Simbad)
Write:	<<[ICC2000] Star A>>
N:	4
Object:	* (SIMBAD class: Star)
Note:	N=4 stars in the field of Ginga 0834-43. Star D is a proposed optical counterpart of Ginga 0834-43.
Ref:	=2000MNRAS.314...87I
by	ISRAEL G.L. , COVINO S., CAMPANA S., POLCARO V.F., ROCHE P., STELLA L., DI PAOLA A., LAZZATI D., MEREGHETTI S., GIALLONGO E., FONTANA A., VERRECCHIA F.
	Mon. Not. R. Astron. Soc., 314, 87-91 (2000)
	The discovery of the optical/IR counterpart of the 12-s transient X-ray pulsar GS 0834-43.
o	Table 3, Fig.2: <[ICC2000] Star A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ICE2013
ICE2013	(Icecube Collaboration, 2013)
Write:	<<ICE2013 NN>>
N:	82
Object:	Neutrino event (SIMBAD class: Transient = Transient Event)
Note:	IceCube observations of N=82 neutrino events. 2013Sci...342E...1I: <ICE2013 NN> (Nos 1-28). 2014PhRvL.113j1101A: <ICE2013 NN> (Nos 29-37) added. 2015ICRC...34.1081K: <ICE2013 NN> (Nos 38-54) added. 2017ICRC...35..981K: <ICE2013 NN> (Nos 55-82) added.
Ref:	=2013Sci...342..947I
by	ICECUBE COLLABORATION
	Science, 342, 947 (2013)
	Evidence for high-energy extraterrestrial neutrinos at the IceCube detector.
o	Table 1: <ICE2013 NN> (Nos 1-28).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ICE2016
ICE2016	(Icecube Collaboration, 2016)
Write:	<<ICE2016 NN>>
N:	36
Object:	Neutrino event (SIMBAD class: Transient = Transient Event)
Note:	IceCube observations of N=36 neutrino events. 2016ApJ...833....3A: <ICE2016 NN> (Nos 1-29). 2017ICRC...35.1005H: <ICE2016 NN> (Nos 30-36) added.
Ref:	=2016ApJ...833....3A
by	AARTSEN M.G. , ABRAHAM K., ACKERMANN M., ADAMS J., AGUILAR J.A., AHLERS M., AHRENS M., ALTMANN D., ANDEEN K., ANDERSON T., ANSSEAU I., ANTON G., ARCHINGER M., ARGUELLES C., AUFFENBERG J., AXANI S., BAI X., BARWICK S.W., BAUM V., BAY R., BEATTY J.J., BECKER TJUS J., BECKER K.-H., BENZVI S., BERGHAUS P., BERLEY D., BERNARDINI E., BERNHARD A., BESSON D.Z., BINDER G., BINDIG D., BISSOK M., BLAUFUSS E., BLOT S., BOHM C., BORNER M., BOS F., BOSE D., BOSER S., BOTNER O., BRAUN J., BRAYEUR L., BRETZ H.-P., BURGMAN A., CARVER T., CASIER M., CHEUNG E., CHIRKIN D., CHRISTOV A., CLARK K., CLASSEN L., COENDERS S., COLLIN G.H., CONRAD J.M., COWEN D.F., CROSS R., DAY M., DE ANDRE J.P.A.M., DE CLERCQ C., DEL PINO ROSENDO E., DEMBINSKI H., DE RIDDER S., DESIATI P., DE VRIES K.D., DE WASSEIGE G., DE WITH M., DEYOUNG T., DIAZ-VELEZ J.C., DI LORENZO V., DUJMOVIC H., DUMM J.P., DUNKMAN M., EBERHARDT B., EHRHARDT T., EICHMANN B., ELLER P., EULER S., EVENSON P.A., FAHEY S., FAZELY A.R., FEINTZEIG J., FELDE J., FILIMONOV K., FINLEY C., FLIS S., FOSIG C.-C., FRANCKOWIAK A., FRIEDMAN E., FUCHS T., GAISSER T.K., GALLAGHER J., GERHARDT L., GHORBANI K., GIANG W., GLADSTONE L., GLAGLA M., GLUSENKAMP T., GOLDSCHMIDT A., GOLUP G., GONZALEZ J.G., GRANT D., GRIFFITH Z., HAACK C., HAJ ISMAIL A., HALLGREN A., HALZEN F., HANSEN E., HANSMANN B., HANSMANN T., HANSON K., HEBECKER D., HEEREMAN D., HELBING K., HELLAUER R., HICKFORD S., HIGNIGHT J., HILL G.C., HOFFMAN K.D., HOFFMANN R., HOLZAPFEL K., HOSHINA K., HUANG F., HUBER M., HULTQVIST K., IN S., ISHIHARA A., JACOBI E., JAPARIDZE G.S., JEONG M., JERO K., JONES B.J.P., JURKOVIC M., KAPPES A., KARG T., KARLE A., KATZ U., KAUER M., KEIVANI A., KELLEY J.L., KEMP J., KHEIRANDISH A., KIM M., KINTSCHER T., KIRYLUK J., KITTLER T., KLEIN S.R., KOHNEN G., KOIRALA R., KOLANOSKI H., KONIETZ R., KOPKE L., KOPPER C., KOPPER S., KOSKINEN D.J., KOWALSKI M., KRINGS K., KROLL M., KRUCKL G., KRUGER C., KUNNEN J., KUNWAR S., KURAHASHI N., KUWABARA T., LABARE M., LANFRANCHI J.L., LARSON M.J., LAUBER F., LENNARZ D., LESIAK-BZDAK M., LEUERMANN M., LEUNER J., LU L., LUNEMANN J., MADSEN J., MAGGI G., MAHN K.B.M., MANCINA S., MANDELARTZ M., MARUYAMA R., MASE K., MAUNU R., McNALLY F., MEAGHER K., MEDICI M., MEIER M., MELI A., MENNE T., MERINO G., MEURES T., MIARECKI S., MOHRMANN L., MONTARULI T., MOULAI M., NAHNHAUER R., NAUMANN U., NEER G., NIEDERHAUSEN H., NOWICKI S.C., NYGREN D.R., OBERTACKE POLLMANN A., OLIVAS A., O'MURCHADHA A., PALCZEWSKI T., PANDYA H., PANKOVA D.V., PEIFFER P., PENEK O., PEPPER J.A., PEREZ DE LOS HEROS C., PIELOTH D., PINAT E., PRICE P.B., PRZYBYLSKI G.T., QUINNAN M., RAAB C., RADEL L., RAMEEZ M., RAWLINS K., REIMANN R., RELETHFORD B., RELICH M., RESCONI E., RHODE W., RICHMAN M., RIEDEL B., ROBERTSON S., RONGEN M., ROTT C., RUHE T., RYCKBOSCH D., RYSEWYK D., SABBATINI L., SANCHEZ HERRERA S.E., SANDROCK A., SANDROOS J., SARKAR S., SATALECKA K., SCHIMP M., SCHLUNDER P., SCHMIDT T., SCHOENEN S., SCHONEBERG S., SCHUMACHER L., SECKEL D., SEUNARINE S., SOLDIN D., SONG M., SPICZAK G.M., SPIERING C., STAHLBERG M., STANEV T., STASIK A., STEUER A., STEZELBERGER T., STOKSTAD R.G., STOSSL A., STROM R., STROTJOHANN N.L., SULLIVAN G.W., SUTHERLAND M., TAAVOLA H., TABOADA I., TATAR J., TENHOLT F., TER-ANTONYAN S., TERLIUK A., TESIC G., TILAV S., TOALE P.A., TOBIN M.N., TOSCANO S., TOSI D., TSELENGIDOU M., TURCATI A., UNGER E., USNER M., VANDENBROUCKE J., VAN EIJNDHOVEN N., VANHEULE S., VAN ROSSEM M., VAN SANTEN J., VEENKAMP J., VEHRING M., VOGE M., VRAEGHE M., WALCK C., WALLACE A., WALLRAFF M., WANDKOWSKY N., WEAVER C., WEISS M.J., WENDT C., WESTERHOFF S., WHELAN B.J., WICKMANN S., WIEBE K., WIEBUSCH C.H., WILLE L., WILLIAMS D.R., WILLS L., WOLF M., WOOD T.R., WOOLSEY E., WOSCHNAGG K., XU D.L., XU X.W., XU Y., YANEZ J.P., YODH G., YOSHIDA S., ZOLL M., (The IceCube Collaboration)
	Astrophys. J., 833, 3-3 (2016)
	Observation and characterization of a cosmic muon neutrino flux from the Northern Hemisphere using six years of IceCube data.
o	Table 4: <ICE2016 NN> (Nos 1-29).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ICE2022
ICE2022	(Icecube Collaboration, 2022)
Write:	<<ICE2022 II-NN>>
N:	35
Object:	Neutrino Event (SIMBAD class: Transient = Transient Event)
Stat:	is completely incorporated in Simbad
Note:	IceCube observations of N=35 neutrino events. See also ICE2016.
Ref:	=2022ApJ...928...50A
by	ABBASI R. , ACKERMANN M., ADAMS J., AGUILAR J.A., AHLERS M., AHRENS M., ALAMEDDINE J.M., ALISPACH C., ALVES A.A.Jr, AMIN N.M., ANDEEN K., ANDERSON T., ANTON G., ARGUELLES C., ASHIDA Y., AXANI S., BAI X., BALAGOPAL V.A., BARBANO A., BARWICK S.W., BASTIAN B., BASU V., BAUR S., BAY R., BEATTY J.J., BECKER K.-H., BECKER TJUS J., BELLENGHI C., BENZVI S., BERLEY D., BERNARDINI E., BESSON D.Z., BINDER G., BINDIG D., BLAUFUSS E., BLOT S., BODDENBERG M., BONTEMPO F., BOROWKA J., BOSER S., BOTNER O., BOTTCHER J., BOURBEAU E., BRADASCIO F., BRAUN J., BRINSON B., BRON S., BROSTEAN-KAISER J., BROWNE S., BURGMAN A., BURLEY R.T., BUSSE R.S., CAMPANA M.A., CARNIE-BRONCA E.G., CHEN C., CHEN Z., CHIRKIN D., CHOI K., CLARK B.A., CLARK K., CLASSEN L., COLEMAN A., COLLIN G.H., CONRAD J.M., COPPIN P., CORREA P., COWEN D.F., CROSS R., DAPPEN C., DAVE P., DE CLERCQ C., DELAUNAY J.J., DELGADO LOPEZ D., DEMBINSKI H., DEOSKAR K., DESAI A., DESIATI P., DE VRIES K.D., DE WASSEIGE G., DE WITH M., DEYOUNG T., DIAZ A., DIAZ-VELEZ J.C., DITTMER M., DUJMOVIC H., DUNKMAN M., DUVERNOIS M.A., DVORAK E., EHRHARDT T., ELLER P., ENGEL R., ERPENBECK H., EVANS J., EVENSON P.A., FAN K.L., FAZELY A.R., FEIGL N., FIEDLSCHUSTER S., FIENBERG A.T., FILIMONOV K., FINLEY C., FISCHER L., FOX D., FRANCKOWIAK A., FRIEDMAN E., FRITZ A., FURST P., GAISSER T.K., GALLAGHER J., GANSTER E., GARCIA A., GARRAPPA S., GERHARDT L., GHADIMI A., GLASER C., GLAUCH T., GLUSENKAMP T., GONZALEZ J.G., GOSWAMI S., GRANT D., GREGOIRE T., GRISWOLD S., GUNTHER C., GUTJAHR P., HAACK C., HALLGREN A., HALLIDAY R., HALVE L., HALZEN F., HA MINH M., HANSON K., HARDIN J., HARNISCH A.A., HAUNGS A., HEBECKER D., HELBING K., HENNINGSEN F., HETTINGER E.C., HICKFORD S., HIGNIGHT J., HILL C., HILL G.C., HOFFMAN K.D., HOFFMANN R., HOKANSON-FASIG B., HOSHINA K., HUANG F., HUBER M., HUBER T., HULTQVIST K., HUNNEFELD M., HUSSAIN R., HYMON K., IN S., IOVINE N., ISHIHARA A., JANSSON M., JAPARIDZE G.S., JEONG M., JIN M., JONES B.J.P., KANG D., KANG W., KANG X., KAPPES A., KAPPESSER D., KARDUM L., KARG T., KARL M., KARLE A., KATZ U., KAUER M., KELLERMANN M., KELLEY J.L., KHEIRANDISH A., KIN K., KINTSCHER T., KIRYLUK J., KLEIN S.R., KOIRALA R., KOLANOSKI H., KONTRIMAS T., KOPKE L., KOPPER C., KOPPER S., KOSKINEN D.J., KOUNDAL P., KOVACEVICH M., KOWALSKI M., KOZYNETS T., KUN E., KURAHASHI N., LAD N., LAGUNAS GUALDA C., LANFRANCHI J.L., LARSON M.J., LAUBER F., LAZAR J.P., LEE J.W., LEONARD K., LESZCZYNSKA A., LI Y., LINCETTO M., LIU Q.R., LIUBARSKA M., LOHFINK E., LOZANO MARISCAL C.J., LU L., LUCARELLI F., LUDWIG A., LUSZCZAK W., LYU Y., MA W.Y., MADSEN J., MAHN K.B.M., MAKINO Y., MANCINA S., MARIS I.C., MARTINEZ-SOLER I., MARUYAMA R., MASE K., McELROY T., McNALLY F., MEAD J.V., MEAGHER K., MECHBAL S., MEDINA A., MEIER M., MEIGHEN-BERGER S., MICALLEF J., MOCKLER D., MONTARULI T., MOORE R.W., MORSE R., MOULAI M., NAAB R., NAGAI R., NAUMANN U., NECKER J., NGUYEN L.V., NIEDERHAUSEN H., NISA M.U., NOWICKI S.C., OBERTACKE POLLMANN A., OEHLER M., OEYEN B., OLIVAS A., O'SULLIVAN E., PANDYA H., PANKOVA D.V., PARK N., PARKER G.K., PAUDEL E.N., PAUL L., PEREZ DE LOS HEROS C., PETERS L., PETERSON J., PHILIPPEN S., PIEPER S., PITTERMANN M., PIZZUTO A., PLUM M., POPOVYCH Y., PORCELLI A., PRADO RODRIGUEZ M., PRICE P.B., PRIES B., PRZYBYLSKI G.T., RAAB C., RAISSI A., RAMEEZ M., RAWLINS K., REA I.C., REHMAN A., REICHHERZER P., REIMANN R., RENZI G., RESCONI E., REUSCH S., RHODE W., RICHMAN M., RIEDEL B., ROBERTS E.J., ROBERTSON S., ROELLINGHOFF G., RONGEN M., ROTT C., RUHE T., RYCKBOSCH D., RYSEWYK CANTU D., SAFA I., SAFFER J., SANCHEZ HERRERA S.E., SANDROCK A., SANDROOS J., SANTANDER M., SARKAR S., SARKAR S., SATALECKA K., SCHAUFEL M., SCHIELER H., SCHINDLER S., SCHMIDT T., SCHNEIDER A., SCHNEIDER J., SCHRODER F.G., SCHUMACHER L., SCHWEFER G., SCLAFANI S., SECKEL D., SEUNARINE S., SHARMA A., SHEFALI S., SILVA M., SKRZYPEK B., SMITHERS B., SNIHUR R., SOEDINGREKSO J., SOLDIN D., SPANNFELLNER C., SPICZAK G.M., SPIERING C., STACHURSKA J., STAMATIKOS M., STANEV T., STEIN R., STETTNER J., STEUER A., STEZELBERGER T., STURWALD T., STUTTARD T., SULLIVAN G.W., TABOADA I., TER-ANTONYAN S., TILAV S., TISCHBEIN F., TOLLEFSON K., TONNIS C., TOSCANO S., TOSI D., TRETTIN A., TSELENGIDOU M., TUNG C.F., TURCATI A., TURCOTTE R., TURLEY C.F., TWAGIRAYEZU J.P., TY B., UNLAND ELORRIETA M.A., VALTONEN-MATTILA N., VANDENBROUCKE J., VAN EIJNDHOVEN N., VANNEROM D., VAN SANTEN J., VERPOEST S., WALCK C., WATSON T.B., WEAVER C., WEIGEL P., WEINDL A., WEISS M.J., WELDERT J., WENDT C., WERTHEBACH J., WEYRAUCH M., WHITEHORN N., WIEBUSCH C.H., WILLIAMS D.R., WOLF M., WOSCHNAGG K., WREDE G., WULFF J., XU X.W., YANEZ J.P., YOSHIDA S., YU S., YUAN T., ZHANG Z., ZHELNIN P., (The IceCube Collaboration)
	Astrophys. J., 928, 50-50 (2022)
	Improved Characterization of the Astrophysical Muon-neutrino Flux with 9.5 Years of IceCube Data.
o	Table 7: <ICE2022 II-NN> (Nos II-1-II-35).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IceCube
IceCube	(IceCube)
Write:	<<IceCube -YYMMDDA>> <<IceCube {HESE\|EHE} NNNNNNNN NNNNNNNN>> <<IceCube YYYYMMDDA>> (not recognised by Simbad, but found in literature) <<IceCube {HESE\|EHE} NNNNNNNN_NNNNNNNN>>
Object:	Neutrino event (SIMBAD class: Transient = Transient Event)
Note:	Neutrino events detected with the IceCube South Pole Neutrino Observatory. IceCube searches for neutrinos from the most violent astrophysical sources: events like exploding stars, gamma-ray bursts, and cataclysmic phenomena involving black holes and neutron stars. The format HESE or EHE NNNNNNNN NNNNNN gives the event number followed by the run number, in the HESE (High Energy Starting Event) program or EHE (Extremely High Energy) program. For more information, visit: http://icecube.wisc.edu/
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ICF2001]
[ICF2001]	(Izotov+Chaffee+Folts+, 2001) (Not yet in Simbad)
Write:	<<[ICF2001] HA Arc>> <<[ICF2001] Loop>> <<[ICF2001] I Zw 18C A>>
N:	1+1+2
Object:	Region (SIMBAD class: Region = Region defined in the Sky)
in source:	ZW I 18 = Mrk 116
Ref:	=2001ApJ...560..222I
by	IZOTOV Y.I. , CHAFFEE F.H., FOLTZ C.B., THUAN T.X., GREEN R.F., PAPADEROS P., FRICKE K.J., GUSEVA N.G.
	Astrophys. J., 560, 222-235 (2001)
	A spectroscopic study of component C and the extended emission around I Zw 18.
o	Component C = [VWH98] HI-C
o	Fig.1: <[ICF2001] HA Arc> N=1, <[ICF2001] Loop> N=1, <[ICF2001] I Zw 18C W> (Nos C, E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ICH2020]
[ICH2020]	(Iodice+Cantiello+Hilker+, 2020)
Write:	<<[ICH2020] Hydra I-UDG NN>> <<[ICH2020] Hydra I-LSB NN>>
N:	12+15
Object:	Poss. Ultra-diffuse G + Poss. LSB Dwarf G (SIMBAD class: LowSurfBrghtG = Low Surface Brightness Galaxy)
Note:	N=12 ultra-diffuse galaxy (UDG) candidates and N=15 low surface brightness (LSB) galaxy candidates in the Hydra I cluster, based on deep observations taken as part of the VST Early-type Galaxy Survey (VEGAS).
in source:	ACO 1060 = NAME Hydra I Cluster
Ref:	=2020A&A...642A..48I
by	IODICE E. , CANTIELLO M., HILKER M., REJKUBA M., ARNABOLDI M., SPAVONE M., GREGGIO L., FORBES D.A., D'AGO G., MIESKE S., SPINIELLO C., LA MARCA A., RAMPAZZO R., PAOLILLO M., CAPACCIOLI M., SCHIPANI P.
	Astron. Astrophys., 642A, 48-48 (2020)
	The first detection of ultra-diffuse galaxies in the Hydra I cluster from the VEGAS survey.
o	Fig. 1, Table 1: <[ICH2020] Hydra I-UDG NN> (Nos 1-12). Fig. 1, Table 2: <ICH2020] Hydra I-LSB NN> (Nos 1-15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ICP2003]
[ICP2003]	(Israel+Covino+Perna+, 2003)
Write:	<<[ICP2003] A>>
N:	2
Object:	? (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra HRC and optical/IR observations of 1RXS J170849.0-400910. N=2 objects in the error circle of 1RXS, A, the brightest, is the most consistent counterpart.
Ref:	=2003ApJ...589L..93I
by	ISRAEL G.L. , COVINO S., PERNA R., MIGNANI R., STELLA L., CAMPANA S., MARCONI G., BONO G., MEREGHETTI S., MOTCH C., NEGUERUELA I., OOSTERBROEK T., ANGELINI L.
	Astrophys. J., 589, 93-96 (2003)
	The infrared counterpart to the anomalous X-ray pulsar 1RXS J170849-400910.
o	Fig.1: <[ICP2003] A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ICP99]
[ICP99]	(Israel+Covino+Polcaro+, 1999)
Write:	<<[ICP99] A>>
N:	9
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=9 stars in the field of 1WGA J1958.2+3232
Ref:	=1999A&A...345L...1I
by	ISRAEL G.L. , COVINO S., POLCARO V.F., STELLA L.
	Astron. Astrophys., 345, 1-4 (1999)
	The identification of the long-period X-ray pulsar 1WGA J1958.2+3232 with a Be-star/X-ray binary.
o	Table 1: <[ICP99] A> (Nos A-E).
Ref:	=2000A&A...359..639U
by	USLENGHI M. , BERGAMINI P., CATALANO S., TOMMASI L., TREVES A.
	Astron. Astrophys., 359, 639-645 (2000)
	Periodic modulation of the optical counterpart of the X-ray pulsator 1WGA J1958.2+3232. A new intermediate polar.
o	Fig.1: <[ICP99] A> (Nos F-I) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ICRF
ICRF	(International Celestial Reference Frame)= (ICRS) = ICRF2
Write:	<<ICRF JHHMMSS.s+DDMMSS>>
N:	212+396+109+3414+4536
Object:	Extragalactic (Rad) (SIMBAD class: Radio = Radio Source)
Note:	The IAU Working Group on Reference Frames has elaborated a reference frame of 610 extragalactic radio-sources to be recommended by the IAU in 1997 as the materialisation of the barycentric J2000.0 International Celestial Reference System (ICRS, see 1995A&A...303..604A). New designations have been given to the objects in the frame following the recommendations of the IAU TG on Designations. The coordinates will be published by April 1997 in a publication issued by the Working Group on Reference Frames. 1998AJ....116..516M: 1st ref. with ICRF objects. See also IERS.
Ref:	=1998AJ....116..516M
by	MA C. , ARIAS E.F., EUBANKS T.M., FEY A.L., GONTIER A.-M., JACOBS C.S., SOVERS O.J., ARCHINAL B.A., CHARLOT P.
	Astron. J., 116, 516-546 (1998)
	The International Celestial Reference Frame as realized by very long baseline interferometry.
o	Tables 3, 4: <ICRF JHHMMSS.s+DDMMSS> = <IERS BHHMM+DDd> N=212+396.
Ref:	=2004AJ....127.3587F
by	FEY A.L. , MA C., ARIAS E.F., CHARLOT P., FEISSEL-VERNIER M., GONTIER A.-M., JACOBS C.S., LI J., MacMILLAN D.S.
	Astron. J., 127, 3587-3608 (2004)
	The second extension of the international celestial reference frame: ICRF-EXT.1.
o	Table 1: <ICRF JHHMMSS.s+DDMMSS> N=109.
Ref:	=2013yCat.1323....0M
by	MA C. , ARIAS F.E., BIANCO G., BOBOLTZ D.A., BOLOTIN S.L., CHARLOT P., ENGELHARDT G., FEY A.L., GAUME R.A., GONTIER A.-M., HEINKELMANN R., JACOBS C.S., KURDUBOV S., LAMBERT S.B., MALKIN Z.M., NOTHNAGEL A., PETROV L., SKURIKHINA E., SOKOLOVA J.R., SOUCHAY J., SOVERS O.J., TESMER V., TITOV O.A., WANG G., ZHAROV V.E., BARACHE C., BOCKMANN S., COLLIOUD A., GIPSON J.M., GORDON D., LYTVYN S.O., MacMILLAN D.S., OJHA R., FEY A.L., GORDON D., JACOBS C.S.
	yCat, 1323, 0 (2013)
	International Celestial Reference Frame 2, ICRF2.
o	<ICRF JHHMMSS.s+DDMMSS> N=3414.
Ref:	=2020A&A...644A.159C
by	CHARLOT P. , JACOBS C.S., GORDON D., LAMBERT S., DE WITT A., BOHM J., FEY A.L., HEINKELMANN R., SKURIKHINA E., TITOV O., ARIAS E.F., BOLOTIN S., BOURDA G., MA C., MALKIN Z., NOTHNAGEL A., MAYER D., MacMILLAN D.S., NILSSON T., GAUME R.
	Astron. Astrophys., 644A, 159-159 (2020)
	The third realization of the International Celestial Reference Frame by very long baseline interferometry.
o	Table 10: <ICRF JHHMMSS.s+DDMMSS> N=4536 = <IERS NHHMM+DDd> N=4536.
=E=	Catalogue in electronic form as I/251
=E=	Catalogue in electronic form as J/AJ/127/3587
=E=	Catalogue in electronic form as I/323
=E=	Catalogue in electronic form as <J/A+A/644/A159/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ICRF2
ICRF2	(International Celestial Reference Frame 2)
====>	Equivalent to: ICRF
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ICRS
ICRS	(International Celestial Reference System)
*****	Avoid the usage of ICRS, prefer ICRF
Origin	of the Acronym: L = Found in the literature
Details on Acronym: ICRS
ICRS	(International Celestial Reference System)
*****	Avoid the usage of ICRS, prefer IERS
Origin	of the Acronym: L (2007KFNT...23..207K)
Details on Acronym: [ICS2009]
[ICS2009]	(Ilbert+Capak+Salvato+, 2009)= (COSMOS)
Write:	<<[ICS2009] NNNNNNN>>
N:	385065
Object:	G (SIMBAD class: Galaxy)
Note:	N=385065 objects as part of the COSMOS-30 photo-z catalog, of accurate photometric redshifts (photo-z) in the COSMOS field. The redshifts are computed with 30 broad, intermediate, and narrowbands covering the UV (Galaxy Evolution Explorer), visible near-IR (NIR; Subaru, Canada–France–Hawaii Telescope (CFHT), United Kingdom Infrared Telescope, and National Optical Astronomy Observatory), and mid-IR (Spitzer/IRAC).
in source:	NAME COSMOS Field
Ref:	=2009ApJ...690.1236I
by	ILBERT O. , CAPAK P., SALVATO M., AUSSEL H., McCRACKEN H.J., SANDERS D.B., SCOVILLE N., KARTALTEPE J., ARNOUTS S., LE FLOC'H E., MOBASHER B., TANIGUCHI Y., LAMAREILLE F., LEAUTHAUD A., SASAKI S., THOMPSON D., ZAMOJSKI M., ZAMORANI G., BARDELLI S., BOLZONELLA M., BONGIORNO A., BRUSA M., CAPUTI K.I., CAROLLO C.M., CONTINI T., COOK R., COPPA G., CUCCIATI O., DE LA TORRE S., DE RAVEL L., FRANZETTI P., GARILLI B., HASINGER G., IOVINO A., KAMPCZYK P., KNEIB J.-P., KNOBEL C., KOVAC K., LE BORGNE J.F., LE BRUN V., FEVRE O.L., LILLY S., LOOPER D., MAIER C., MAINIERI V., MELLIER Y., MIGNOLI M., MURAYAMA T., PELLO R., PENG Y., PEREZ-MONTERO E., RENZINI A., RICCIARDELLI E., SCHIMINOVICH D., SCODEGGIO M., SHIOYA Y., SILVERMAN J., SURACE J., TANAKA M., TASCA L., TRESSE L., VERGANI D., ZUCCA E.
	Astrophys. J., 690, 1236-1249 (2009)
	COSMOS photometric redshifts with 30-Bands for 2-°^{2}.
o	<[ICS2009] NNNNNNN> N=385065 among (Nos 26310-1993775).
=E=	Catalogue in electronic form as <J/ApJ/690/1236/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ICS96]
[ICS96]	(Iovino+Clowes+Shaver, 1996)
Write:	<<[ICS96] HHMMSS.s+DDMMSS>>
N:	1555
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Stat:	is completely incorporated in Simbad
Ref:	=1996A&AS..119..265I
by	IOVINO A. , CLOWES R., SHAVER P.
	Astron. Astrophys., Suppl. Ser., 119, 265-269 (1996)
	A large sample of objective prism quasar candidates.
o	Table 3: <[ICS96] HHMMSS.s+DDMMSS> N=1592
=E=	Catalogue in electronic form as J/A+AS/119/265
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ICS99]
[ICS99]	(Israel+Covino+Stella+, 1999)
Write:	<<[ICS99] A>>
N:	12
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations: (Nos A-L), stars in the error box of 1RXS J170849.0-400910.
Ref:	=1999ApJ...518L.107I
by	ISRAEL G.L. , COVINO S., STELLA L., CAMPANA S., HABERL F., MEREGHETTI S.
	Astrophys. J., 518, 107-110 (1999)
	Further evidence that 1RXS J170849.0-400910 is an anomalous X-ray pulsar.
o	Fig.3, Table 1: <[ICS99] A> (Nos A-L).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IDC2015]
[IDC2015]	(Irwin+Dupke+Carrasco+, 2015)
Write:	<<[IDC2015] NNNN>>
N:	78
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Gemini GMOS-N spectroscopic observations of N=78 galaxies of the Cheshire Cat gravitational lens system. Use of archival HST WFC3 data.
in source:	NAME Cheshire Cat Group
Ref:	=2015ApJ...806..268I
by	IRWIN J.A. , DUPKE R., CARRASCO E.R., MAKSYM W.P., JOHNSON L., WHITE III R.E.
	Astrophys. J., 806, 268 (2015)
	The Cheshire Cat gravitational lens: the formation of a massive fossil group.
o	Table 1: <[IDC2015] NNNN> (Nos 1-2184).
=E=	Catalogue in electronic form as J/ApJ/806/268
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IDCS
IDCS	(Spitzer IRAC Distant Cluster Survey)
Write:	<<IDCS JHHMM.m+DDMM>>
N:	1 (SIMBAD class: ClG = Cluster of Galaxies)
Note:	Search for galaxy clusters in the Spitzer Deep, Wide-Field Survey (SDWFS).
Ref:	=2012ApJ...753..162B
by	BRODWIN M. , GONZALEZ A.H., STANFORD S.A., PLAGGE T., MARRONE D.P., CARLSTROM J.E., DEY A., EISENHARDT P.R., FEDELI C., GETTINGS D., JANNUZI B.T., JOY M., LEITCH E.M., MANCONE C., SNYDER G.F., STERN D., ZEIMANN G.
	Astrophys. J., 753, 162 (2012)
	IDCS J1426.5+3508: Sunyaev-Zel'dovich measurement of a massive infrared-selected cluster at z = 1.75.
o	<IDCS JHHMM.m+DDMM> N=1
Ref:	=2012ApJ...753..163G
by	GONZALEZ A.H. , STANFORD S.A., BRODWIN M., FEDELI C., DEY A., EISENHARDT P.R.M., MANCONE C., STERN D., ZEIMANN G.
	Astrophys. J., 753, 163 (2012)
	IDCS J1426.5+3508: cosmological implications of a massive, strong lensing cluster at z = 1.75.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IDF98]
[IDF98]	(Izumiura+Deguchi+Fujii, 1998)
Write:	<<[IDF98] SiO LLL.lll-B.bbb N>>
N:	4+7+3
Object:	SiO Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	Survey of stellar maser sources towards the Galactic Center in SiO lines.
in source:	NAME Gal Center
Ref:	=1998ApJ...494L..89I
by	IZUMIURA H. , DEGUCHI S., FUJII T.
	Astrophys. J., 494, 89-92 (1998)
	SiO maser forest at the Galactic Center.
o	Table 1: <[IDF98] SiO 359.933-0.046 N> N=4, <[IDF98] SiO 359.944-0.046 N> N=7, <[IDF98] SiO 359.955-0.046 N> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IDF99]
[IDF99]	(Izumiura+Deguchi+Fujii, 1999) (Not yet in Simbad)
Write:	<<[IDF99] HHMMm+DDMM>>
N:	69+86+124
Object:	SiO Maser (SIMBAD class: Maser)
Note:	N=69+86+124 SiO maser sources in IRAS sources.
Ref:	=1999ApJS..125..257I
by	IZUMIURA H. , DEGUCHI S., FUJII T., KAMEYA O., MATSUMOTO S., NAKADA Y., OOTSUBO T., UKITA N.
	Astrophys. J., Suppl. Ser., 125, 257-276 (1999)
	SiO maser survey of the galactic disk IRAS sources. I. 15°<l<25°, near end of the Galactic Bar.
o	Table 1: <[IDF99] HHMMm+DDMM> N=69.
Ref:	=2000ApJS..128..571D
by	DEGUCHI S. , FUJII T., IZUMIURA H., KAMEYA O., NAKADA Y., NAKASHIMA J.-I., OOTSUBO T., UKITA N.
	Astrophys. J., Suppl. Ser., 128, 571-595 (2000)
	SiO maser survey of the galactic disk IRAS sources. II. \|l\|≤3° and \|b\|≤3°, the Galactic Center area.
o	Table 2: <[IDF99] HHMMm+DDMM> N=86.
Ref:	=2000ApJS..130..351D
by	DEGUCHI S. , FUJII T., IZUMIURA H., KAMEYA O., NAKADA Y., NAKASHIMA J.-I.
	Astrophys. J., Suppl. Ser., 130, 351-379 (2000)
	SiO maser survey of the Galactic disk IRAS sources. III. -10°< l<15° and \|b\|≤3°, a central part of the Galaxy.
o	Table 1: <[IDF99] HHMMm+DDMM> N=124.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IDJ2003]
[IDJ2003]	(Israel+De Graauw+Johansson+, 2003)
Write:	<<[IDJ2003] NN>>
N:	29
Object:	CO Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
in source:	Magellanic Clouds:LMC:LHA 120-N 11 = LHA 120-N 11
Ref:	=2003A&A...401...99I
by	ISRAEL F.P. , DE GRAAUW T., JOHANSSON L.E.B., BOOTH R.S., BOULANGER F., GARAY G., KUTNER M.L., LEQUEUX J., NYMAN L.-A., RUBIO M.
	Astron. Astrophys., 401, 99-111 (2003)
	Results of the ESO-SEST Key Programme on CO in the Magellanic Clouds. IX. The giant LMC HII region complex N 11.
o	Table 1: <[IDJ2003] NN> (Nos 1-29).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IDK
IDK	(Irwin+Demers+Kunkel)
Write:	<<IDK N>> <<IDK ANNNA>>
N:	6+28
Object:	Blue * Assoc. + * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Table III: (Nos 1-6), N=6 associations of stars. Tables IV, V: N=28 yellow and blue stars in sequences 'A' (Nos A-P, O missing).
in source:	Magellanic Clouds:Magellanic Bridge = Magellanic Bridge
Ref:	=1990AJ.....99..191I
by	IRWIN M.J. , DEMERS S., KUNKEL W.E.
	Astron. J., 99, 191-200 (1990)
	A blue stellar link between the Magellanic Clouds.
o	Table III: <IDK N> N=6, Tables IV, V: <IDK ANNNA> N=28
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IDS
IDS	(Index catalog of Double *)= (USNO)
Write:	<<IDS HHMMm+DDMMAAAA>>
N:	about 64000
Object:	(SIMBAD class: = Double or Multiple Star)
Note:	Format: 1900 coord. Also found in the literature with the formats HHMM.mNDDMMA and HHMM.mSDDMMA instead of '+' and '-'. Superseded by WDS. See also PMSC.
Ref:	=1963IDS...C......0J
by	JEFFERS H.M. , VAN DEN BOS W.H., GREEBY F.M.
	Publ. Lick Obs. 21,part 1,1963, 0-None (1963)
	Index catalogue of visual double stars, 1961.0.
o	part 1 (263pp) + part part 2 (804pp).
o	<IDS HHMMm+DDMMAAAA> N=about 64000.
Details on Acronym: [IDS2000]
[IDS2000]	(Ivison+Dunlop+Smail+, 2000)= (HzRG)
Write:	<<[IDS2000] 850.N>> <<[IDS2000] 850.N KN>>
N:	5+7
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=5 850 mu.m sources in the radio galaxy 4C 41.17, format '850.N'. Map Fig.1. Fig.3, table 2: possible counterparts of the submm sources, format '850.N KN'.
Ref:	=2000ApJ...542...27I
by	IVISON R.J. , DUNLOP J.S., SMAIL I., DEY A., LIU M.C., GRAHAM J.R.
	Astrophys. J., 542, 27-34 (2000)
	An excess of submillimeter sources near 4C 41.17: a candidate protocluster at z = 3.8?.
o	Table 1: <[IDS2000] 850.N> (Nos 850.1 to 850.5). Table 2, Fig.3: <[IDS2000] 850.N KN> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IDSCL
IDSCL	(IfA Deep Survey Cluster)
*****	Avoid the usage of IDSCL, prefer [FSL2005]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IE
IE	(Erroneously printed for 1E)
*****	Avoid the usage of IE, prefer 1E
Details on Acronym: [IEF2000]
[IEF2000]	(Iwasawa+Ettori+Fabian+, 2000) (Not yet in Simbad)
Write:	<<[IEF2000] 3C 353 W>> <<[IEF2000] 3C 353 Wa>> <<[IEF2000] 3C 353 WWa>> <<[IEF2000] gN>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Note:	ASCA observations of 3C 353, one of the bright galaxy in the central part of ZwCl 1718-0108: 3 X-ray components are indicated (N, C, S) in Fig.1, 1 west-plume (Wp) and 1 north-east plume (NWp) in Fig.2. Fig.4, Table 4: N=3 other bright galaxies in the central part of ZwCl 1718-0108 (Nos g1-g3).
in source:	ZwCl 1718-0108
Ref:	=2000MNRAS.313..515I
by	IWASAWA K. , ETTORI S., FABIAN A.C., EDGE A.C., EBELING H.
	Mon. Not. R. Astron. Soc., 313, 515-523 (2000)
	Zw 1718.1-0108: a highly disturbed galaxy cluster at low Galactic latitude.
o	Table 4: g1 = 2MASX J17204075-0108573, g2 = 2MASX J17204089-0111573, g3 = LEDA 1126470.
o	Figs 1, 2: <[IEF2000] 3C 353 W> (Nos N, C, S), <[IEF2000] 3C 353 Wp> N=1, <[IEF2000] 3C 353 NWp> N=1. Table 4: <[IEF2000] gN> (Nos g1-g3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IER2010]
[IER2010]	(Israel+Erben+Reiprich+, 2010)
Write:	<<[IER2010] GN>> <<[IER2010] PNN>> <<[IER2010] JHHMMSS.s+DDMMSS>>
N:	4+10+2
Object:	G + Peak + Poss. Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	MMT Megacam observations of the cluster ClG J0030+2618.
in source:	ClG J0030+2618
Ref:	=2010A&A...520A..58I
by	ISRAEL H. , ERBEN T., REIPRICH T.H., VIKHLININ A., HILDEBRANDT H., HUDSON D.S., McLEOD B.A., SARAZIN C.L., SCHNEIDER P., ZHANG Y.-Y.
	Astron. Astrophys., 520A, 58-58 (2010)
	The 400d galaxy cluster survey weak lensing programme. I. MMT/Megacam analysis of CL0030+2618 at z = 0.50.
o	Fig. 1, Table 2: <[IER2010] GN> (Nos G1-G4). Fig. 8, Table 4: <[IER2010] PNN> (Nos P1-P10). Fig. 1, Paragr. 5.4: <[IER2010] JHHMMSS.s+DDMMSS> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IERO
IERO	(IRAC-selected Extremely Red Object)
Write:	<<IERO NN>>
N:	17
Object:	Extremely Red Obj. (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Data form the Infrared Array Camera (IRAC) on the Spitzer Space Telescope taken for the GOODS survey are used to identify high redshift extremely red objects in the HUDF.
in source:	NAME HUDF
Ref:	=2004ApJ...616...63Y
by	YAN H. , DICKINSON M., EISENHARDT P.R.M., FERGUSON H.C., GROGIN N.A., PAOLILLO M., CHARY R.-R., CASERTANO S., STERN D., REACH W.T., MOUSTAKAS L.A., FALL S.M.
	Astrophys. J., 616, 63-70 (2004)
	High-redshift extremely red objects in the Hubble space telescope Ultra Deep Field revealed by the GOODS infrared array camera observations.
o	Table 1: <IERO NN> (Nos 1-17).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IERS
IERS	(International Earth Rotation Service)
Write:	<<IERS BHHMM+DDd>>
Object:	Extragalactic (Rad) (SIMBAD class: Radio = Radio Source)
Note:	1998AJ....116..516M: 1st ref. with ICRF objects. See also ICRF 2010A&A...520A.113B: search for additional suitable radio sources for aligning the Gaia and VLBI frames.
Ref:	=1998AJ....116..516M
by	MA C. , ARIAS E.F., EUBANKS T.M., FEY A.L., GONTIER A.-M., JACOBS C.S., SOVERS O.J., ARCHINAL B.A., CHARLOT P.
	Astron. J., 116, 516-546 (1998)
	The International Celestial Reference Frame as realized by very long baseline interferometry.
o	Tables 3, 4: <ICRF JHHMMSS.s+DDMMSS> = <IERS BHHMM+DDd> N=212+396.
Ref:	=2010A&A...520A.113B
by	BOURDA G. , CHARLOT P., PORCAS R.W., GARRINGTON S.T.
	Astron. Astrophys., 520A, 113-113 (2010)
	VLBI observations of optically-bright extragalactic radio sources for the alignment of the radio frame with the future Gaia frame. I. Source detection.
o	Tables 3-4: <IERS HHMM+DDd> N=398+49.
=E=	Catalogue in electronic form as I/251
=E=	Catalogue in electronic form as J/A+A/520/A113
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [IF2012]
[IF2012]	(Ioannidis+Froebrich, 2012) (Not yet in Simbad)
Write:	<<[IF2012] MHO NNNNa>>
N:	?
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	UKIRT observations of jets and outflows in the Serpens and Aquila regions, as part of the UKIRT Wide Field Infrared Survey for H2 (UWISH2).
in source:	NAME Ser Region
in source:	NAME Aql Region
Ref:	=2012MNRAS.421.3257I
by	IOANNIDIS G. , FROEBRICH D.
	Mon. Not. R. Astron. Soc., 421, 3257-3265 (2012)
	YSO jets in the Galactic plane from UWISH2 - I. MHO catalogue for Serpens and Aquila.
o	Table A1: <MHO NNNN> (Nos 2201-2212, 2244-2299, 2436-2456, 3200-3246) added. Table B1: <[IF2012] MHO NNNNa> N=141.
=E=	Catalogue in electronic form as <J/MNRAS/421/3257/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IF2019]
[IF2019]	(Imara+Faesi, 2019)
Write:	<<[IF2019] He 2-10 NNN>>
N:	119
Object:	Giant MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	ALMA band 3 12CO(1-0) observations of N=119 giant molecular clouds in the dwarf galaxy Hen 2-10.
in source:	Hen 2-10
Ref:	=2019ApJ...876..141I
by	IMARA N. , FAESI C.M.
	Astrophys. J., 876, 141-141 (2019)
	ALMA observations of giant molecular clouds in the starburst dwarf galaxy Henize 2-10.
o	Table 3: <[IF2019] He 2-10 NNN> (Nos 1-119).
=E=	Catalogue in electronic form as <J/ApJ/876/141/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IF76]
[IF76]	(Israel+Felli, 1976)
Write:	<<[IF76] NN>>
N:	43
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Westerbork Synthesis Radio telescope observations. Radio-sources in the field of Sh 2-80 (PN M 1-67), Sh 2-105, Sh 2-188, Sh 2-298 (NGC 2359).
Ref:	=1976A&A....50...47I
by	ISRAEL F.P. , FELLI M.
	Astron. Astrophys., 50, 47-53 (1976)
	Aperture synthesis radio observations of three filamentary nebulae.
o	Table 4: <[IF76] NN> (Nos 1-43).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IF78]
[IF78]	(Israel+Felli, 1978)
Write:	<<[IF78] S106 A>> <<[IF78] S235 NN>>
N:	3+11
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Table 4: N=3 regions (Nos A-C) in Sh 2-106. Table 5: N=11 regions (Nos 1-11) in Sh 2-235
in source:	SH 2-106
in source:	SH 2-235
Ref:	=1978A&A....63..325I
by	ISRAEL F.P. , FELLI M.
	Astron. Astrophys., 63, 325-334 (1978)
	Aperture synthesis observations of galactic HII regions. VIII. S 106 and S 235: Regions of star formation.
o	Table 4: <[IF78] S106 A> (Nos A-C). Table 5: <[IF78] S235 NN> (Nos 1-11)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IfAH-alpha
IfAH-alpha	(Institute for Astron. in Hawaii, H-alpha obj.)
*****	Avoid the usage of IfAH-alpha, prefer IfAHA
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IfAHA
IfAHA	(Institute for Astron. in Hawaii, H-alpha obj.)= (IfAH-alpha) = (IH-alpha)
Write:	<<IfAHA NNN>>
N:	821
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Note:	H-alpha emission stars: (Nos 1-102) in IC 348. (Nos 104-186) in IC 5146. (Nos 187-222) in NGC 1579. (Nos 223-491) in NGC 1164. (Nos 492-621) in NGC 2362. (Nos 622-685) in LDN 988. (Nos 686-762) in IC 1274. (Nos 763-821) in NGC 7129.
in source:	IC 348
in source:	IC 5146
in source:	NGC 1579
in source:	LDN 988
in source:	IC 1274
in source:	NGC 7129
Ref:	=1996A&A...310..456P
by	PREIBISCH T. , ZINNECKER H., HERBIG G.H.
	Astron. Astrophys., 310, 456-473 (1996)
	ROSAT X-ray observations of the young cluster IC 348.
o	Table 1: <[PZH96] NNN> (Nos 1-116). Table 5: <IfAHA NN> N=31 among (Nos 5-58)
Ref:	=1998ApJ...497..736H
by	HERBIG G.H.
	Astrophys. J., 497, 736-758 (1998)
	The young cluster IC 348.
o	Table 1: <Cl* IC 348 H NNN> (Nos 1-261). Tables 1, 6: <IfAHA NNN> (Nos 59-102).
Ref:	=2002AJ....123..304H
by	HERBIG G.H. , DAHM S.E.
	Astron. J., 123, 304-327 (2002)
	The young cluster IC 5146.
o	Tables 1, 2: <[HD2002] Star NNN> (Nos 1-380, 400-710). Tables 1, 2: <IfAHA NNN> (Nos 104-186) added. Table 10: <[HD2002] IR N> (Nos 1-7). Table 11: <[HD2002] Cloud A> (Nos A-D).
Ref:	=2004AJ....128.1233H
by	HERBIG G.H. , ANDREWS S.M., DAHM S.E.
	Astron. J., 128, 1233-1253 (2004)
	LkHα 101 and the young cluster in NGC 1579.
o	Table 1: <[HAD2004] NGC 1579 NNN> (Nos 1-325). Table 4: <[HAD2004] LDN 1482 A> (Nos A-H). Table 2: <IfAHA NNN> (Nos 187-222) added.
Ref:	=2005AJ....129..829D
by	DAHM S.E. , SIMON T.
	Astron. J., 129, 829-855 (2005)
	The T Tauri star population of the young cluster NGC 2264.
o	Table 1: <Cl* NGC 2264 DS NNN> (Nos 1-490). Table 1: <IfAHA NNN> (Nos 223-491) added.
Ref:	=2005AJ....130.1805D
by	DAHM S.E.
	Astron. J., 130, 1805-1828 (2005)
	The young cluster NGC 2362.
o	Table 1, col(1): <Cl* NGC 2362 D NNN> (Nos 1-130) = <IfAHA NNN> (Nos 492-621) added.
Ref:	=2006AJ....131.1530H
by	HERBIG G.H. , DAHM S.E.
	Astron. J., 131, 1530-1543 (2006)
	The pre-main-sequence population of L988.
o	Table 3: <IfAHA NNN> (Nos 622-685) added.
Ref:	=2012AJ....143....3D
by	DAHM S.E. , HERBIG G.H., BOWLER B.P.
	Astron. J., 143, 3 (2012)
	The young cluster in IC 1274.
o	Table 3: <IfAHA NNN> (Nos 686-762) added.
Ref:	=2015AJ....149..200D
by	DAHM S.E. , HILLENBRAND L.A.
	Astron. J., 149, 200 (2015)
	An optical survey of the partially embedded young cluster in NGC 7129.
o	S3-U1350 is a probable misprint for S2-U1350.
o	Table 1: <IfAHA NNN> (Nos 763-821) added. Table 3: <[DH2015] NN> (Nos 1-72). Table 4: <[DH2015] JHHMMSS.ss+DDMMSS.s> N=2435.
=E=	Catalogue in electronic form as J/AJ/123/304
=E=	Catalogue in electronic form as J/AJ/128/1233
=E=	Catalogue in electronic form as J/AJ/129/829
=E=	Catalogue in electronic form as J/AJ/130/1805
=E=	Catalogue in electronic form as J/AJ/131/1530
=E=	Catalogue in electronic form as <J/AJ/143/3/>
=E=	Catalogue in electronic form as J/AJ/149/200
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [IFG2001]
[IFG2001]	(Im+Faber+Gebhardt+, 2001)
Write:	<<[IFG2001] NN>> <<[IFG2001] FFN-xxyy>>
N:	10
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations. N=10 Blue Spheroid Candidates (BSC). In the format 'FF' stands for the subfield number, 'N' for the wfpc2 chip number, 'xxyy' for the coordinates in units of 10 pixels. Images in Fig.2.
Ref:	=2001AJ....122..750I
by	IM M. , FABER S.M., GEBHARDT K., KOO D.C., PHILLIPS A.C., SCHIAVON R.P., SIMARD L., WILLMER C.N.A.
	Astron. J., 122, 750-763 (2001)
	Are there blue, massive E/S0 galaxies at z<1? Kinematics of blue spheroidal galaxy candidates.
o	p.762: galaxies 084-1138, 093-3251, hd4-241-1, hd2-251-0, not identified.
o	Table 1: <[IFG2001] NN> (Nos 1-10) = <[IFG2001] FFN-xxyy> N=10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IFH94]
[IFH94]	(Infante+Fouque+Hertling+, 1994)
Write:	<<[IFH94] NNN>> <<[IFH94] A>>
N:	12+13
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Table 1: N=12 galaxies in ClG 0017-20, among 213, format 'NNN'. N=13 galaxies used as standards, among (Nos A-Y). Table 3: galaxies in ClG 0500-24 (ACO S 506), designated as [G90].
in source:	ClG 0017-20
Ref:	=1994A&A...289..381I
by	INFANTE L. , FOUQUE P., HERTLING G., WAY M.J., GIRAUD E., QUINTANA H.
	Astron. Astrophys., 289, 381-393 (1994)
	The medium redshift clusters CL 0017-20 and CL 0500-24.
o	Table 1: letters 'n', 'c' are not part of format. Table 3: '[G90] A' or [G90] NN'
o	Table 1: <[IFH94] NNN> N=12 among 213, <[IFH94] A> N=13 among (Nos A-Y)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IFK98]
[IFK98]	(Impey+Falco+Kochanek+, 1998)
Write:	<<[IFK98] GNN>>
N:	15
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST observations of the gravitational lens PG 1115+080. N=15 galaxies members of a nearby group (Nos G1-G15). (Nos G1-G4) are identical to [YDG81] (Nos G1-G4). Map in Fig.2. See also [YDG81].
Ref:	=1998ApJ...509..551I
by	IMPEY C.D. , FALCO E.E., KOCHANEK C.S., LEHAR J., McLEOD B.A., RIX H.-W., PENG C.Y., KEETON C.R.
	Astrophys. J., 509, 551-560 (1998)
	An infrared EINSTEIN ring in the gravitational lens PG 1115+080.
o	lens galaxy = [YDG81] G, A1/A2 = [YDG81] QSO 1115+080 AN.
o	Table 4: <[IFK98] GNN> (Nos G1-G15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IFM-B
IFM-B	(Ivanov+Freedman+Madore, Blue)
Write:	<<IFM-B NNNNa>>
N:	2112+35
Object:	Blue Supergiant (SIMBAD class: Star)
Note:	Table 2: N=2112 blue supergiants, among (Nos 1-2126). An unpublished version of the catalogue has added 35 objects. See also IFM-R
Ref:	=1993ApJS...89...85I
by	IVANOV G.R. , FREEDMAN W.L., MADORE B.F.
	Astrophys. J., Suppl. Ser., 89, 85-122 (1993)
	A catalog of blue and red supergiants in M33.
o	Table 2: <IFM-B NNNNa> N=2112 among (Nos 1-2126). Table 3: <IFM-R NNN> N=389 among (Nos 1-391).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IFM-R
IFM-R	(Ivanov+Freedman+Madore, Red)
Write:	<<IFM-R NNN>>
N:	389
Object:	Red Supergiant (SIMBAD class: Star)
Note:	Table 3: N=389 red supergiants among (Nos 1-391). See also IFM-B
Ref:	=1993ApJS...89...85I
by	IVANOV G.R. , FREEDMAN W.L., MADORE B.F.
	Astrophys. J., Suppl. Ser., 89, 85-122 (1993)
	A catalog of blue and red supergiants in M33.
o	Table 2: <IFM-B NNNNa> N=2112 among (Nos 1-2126). Table 3: <IFM-R NNN> N=389 among (Nos 1-391).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [IFO88]
[IFO88]	(Iwata+Fukui+Ogawa, 1988)
Write:	<<[IFO88] A>>
N:	4
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Table 2: N=4 NH3 clumps in NGC 2071N
in source:	NGC 2071N
Ref:	=1988ApJ...325..372I
by	IWATA T. , FUKUI Y., OGAWA H.
	Astrophys. J., 325, 372-381 (1988)
	A molecular line study of a bipolar outflow object NGC 2071 - north in L 1630.
o	Table 2: <[IFO88] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IG
IG	(Isolated pairs of G)
*****	Avoid the usage of IG, prefer K73
Origin	of the Acronym: L = Found in the literature
Details on Acronym: IG VV
IG VV	(Interacting G, Vorontsov-Vel'yaminov)
*****	Avoid the usage of IG VV, prefer VV
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [IG95]
[IG95]	(Ibata+Gilmore, 1995)
Write:	<<[IG95] NNN-NN>>
N:	1509
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	On Microfiche: format 'NNN-NN', about 1500 stars (format 'NNN') in regions Nos 01 to 04, 10 and 16 (format 'NN')
Ref:	=1995MNRAS.275..591I
by	IBATA R.A. , GILMORE G.
	Mon. Not. R. Astron. Soc., 275, 591-None (1995)
	The outer regions of the Galactic Bulge: I. Observations.
o	<[IG95] NNN-NN> N=1509
=E=	Catalogue in electronic form as J/MNRAS/275/591
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IGAPS
IGAPS	(INT (Isaac Newton Telescope) Galactic Plane Surveys)
Write:	<<IGAPS JHHMMSS.ss+DDMMSS.s>>
N:	about 300 million
Object:	* (SIMBAD class: Star)
Note:	The catalogue associated with this acronym would contain the next IPHAS release, as merged with the photometry from the UVEX survey (for which this will be the first release). The photometric magnitudes provided for point sources are in the i, H-alpha, r (2 different dates of observation), g and U_RGO filters. The astrometry has been placed in the Gaia DR2 frame. Galactic co-ordinates will also be provided. ref=Barentsen et al 2014MNRAS.444.3230B (previous IPHAS release) ref=Monguio et al 2019 MNRAS or A&A
Notes:	Preliminary contact has been made with CDS about hosting this catalogue. The example designations/coords are copied across from IPHAS DR2.
Auth.:	Janet Drew University of Hertfordshire
=E=	Catalogue in electronic form as <V/165/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: IGC
IGC	(Intracluster Globular Cluster)
*****	Avoid the usage of IGC, prefer [WCD2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [IGD2007]
[IGD2007]	(Ivison+Greve+Dunlop+, 2007)
Write:	<<[IGD2007] Radio JHHMMSS.sss+DDMMSS.ss>> <<[IGD2007] MIR JHHMMSS.ss+DDMMSS.s>>
N:	86+72+109+56
Object:	(Rad) + (Mid-IR) (SIMBAD class: Radio = Radio Source)
Note:	SCUBA HAlf Degree Extragalactic Survey: Identification of radio and MIR possible counterparts to [CCM2006] galaxies. Use of archival VLA 1.4GHz observations.
in source:	NAME Lockman Hole
Ref:	=2007MNRAS.380..199I
by	IVISON R.J. , GREVE T.R., DUNLOP J.S., PEACOCK J.A., EGAMI E., SMAIL I., IBAR E., VAN KAMPEN E., ARETXAGA I., BABBEDGE T., BIGGS A.D., BLAIN A.W., CHAPMAN S.C., CLEMENTS D.L., COPPIN K., FARRAH D., HALPERN M., HUGHES D.H., JARVIS M.J., JENNESS T., JONES J.R., MORTIER A.M.J., OLIVER S., PAPOVICH C., PEREZ-GONZALEZ P.G., POPE A., RAWLINGS S., RIEKE G.H., ROWAN-ROBINSON M., SAVAGE R.S., SCOTT D., SEIGAR M., SERJEANT S., SIMPSON C., STEVENS J.A., VACCARI M., WAGG J., WILLOTT C.J.
	Mon. Not. R. Astron. Soc., 380, 199-228 (2007)
	The SCUBA HAlf Degree Extragalactic Survey - III. Identification of radio and mid-infrared counterparts to submillimetre galaxies.
o	Tables 1-2: <[IGD2007] Radio JHHMMSS.sss+DDMMSS.ss> N=86+72. Tables 3-4: <[IGD2007] MIR JHHMMSS.ss+DDMMSS.s> N=109+56.
=E=	Catalogue in electronic form as J/MNRAS/380/199
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IGF2000]
[IGF2000]	(Ivezic+Goldston+Finlator+, 2000)
Write:	<<[IGF2000] NNN>>
N:	148
Object:	Poss. RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Stat:	is completely incorporated in Simbad
Note:	N=148 candidates RR Lyrae stars in the SDSS survey.
Ref:	=2000AJ....120..963I
by	IVEZIC Z. , GOLDSTON J., FINLATOR K., KNAPP G.R., YANNY B., McKAY T.A., AMROSE S., KRISCIUNAS K., WILLMAN B., ANDERSON S., SCHABER C., ERB D., LOGAN C., STUBBS C., CHEN B., NEILSEN E., UOMOTO A., PIER J.R., FAN X., GUNN J.E., LUPTON R.H., ROCKOSI C.M., SCHLEGEL D., STRAUSS M.A., ANNIS J., BRINKMANN J., CSABAI I., DOI M., FUKUGITA M., HENNESSY G.S., HINDSLEY R.B., MARGON B., MUNN J.A., NEWBERG H.J., SCHNEIDER D.P., SMITH J.A., SZOKOLY G.P., THAKAR A.R., VOGELEY M.S., WADDELL P., YASUDA N., YORK D.G., (The SDSS Collaboration)
	Astron. J., 120, 963-977 (2000)
	Candidate RR Lyrae stars found in Sloan Digital Sky Survey commissioning data.
o	Table 2: <[IGF2000] NNN> (Nos 1-148).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IGGC
IGGC	(Inner Galaxy Gas Clump) (Not yet in Simbad)
Write:	<<IGGC NNN>>
N:	30
Object:	Galaxy Gas Clump (SIMBAD class: PartofG = Part of a Galaxy)
Note:	In preparation. The Antarctic Submm Telescope/Remote Observatoryhas recently completed a 5 square degree survey of the inner few degrees of the galactic plane in a variety of submm lines. In the process authors have identified a series of emission sources that have not previously been observed at these frequencies.
Auth.:	MARTIN C.L.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [IGI95]
[IGI95]	(Ibata+Gilmore+Irwin, 1995)
Write:	<<[IGI95] CN>>
N:	4
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Note:	format 'CN' where the letter 'C' stands for Carbon, as found in 1996NewA....1...57W ([WIC96])
in source:	NAME SDG = NAME Sgr Dwarf Galaxy
Ref:	=1995MNRAS.277..781I
by	IBATA R.A. , GILMORE G., IRWIN M.J.
	Mon. Not. R. Astron. Soc., 277, 781-800 (1995)
	Sagittarius : the nearest dwarf galaxy.
o	Table 1: <[IGI95] CN> (Nos C1-C4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IGR
IGR	(INTEGRAL Gamma-Ray source)
Write:	<<IGR JHHMMm+DDMM>>
N:	about 2000
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	The INTEGRAL satellite is ESA's gamma-ray observatory mission, in orbit since 2002. It contains four instruments: a gamma-ray imager (IBIS), a gamma ray spectrometer (SPI), an X-ray monitor (JEM-X) and an optical monitor (OMC). Due to its unprecedented sensitivity, the large field of view of the instruments, and in particular the good imaging performance of the IBIS instrument, INTEGRAL regularly discovers new high energy (gamma-ray) sources. Catalogs of new sources are being published (e.g. 2004ApJ...607L..33B), while many individual detections are reported as Astronomer's Telegrams (http://www.astronomerstelegram.org). Observers who discover a new source in their data are also requested to use the IGR designation. More about INTEGRAL can be found on the following web sites: http://www.rssd.esa.int/Integral http://isdc.unige.ch 2003IAUC.8063....3C : first ref. with IGR object, and the only one listed here.
Ref:	=2003IAUC.8063....3C
by	COURVOISIER T.J.-L. , WALTER R., RODRIGUEZ J., BOUCHET L., LUTOVINOV A.A.
	IAU Circ., 8063, 3-None (2003)
	IGR J16318-4848.
o	<IGR JHHMMm+DDMM> N=1.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: IGRACS
IGRACS	(Not yet in Simbad)
Write:	<<IGRACS YYMMDD.ddddd>>
N:	about 5000
Object:	gB (SIMBAD class: gammaBurst = Gamma-ray Burst)
Note:	This acronym will be used to identify gamma-ray bursts detected by the anticoincidence (ACS) shield of the INTEGRAL spectrometer. The ACS provides all-sky lightcurves with a resolution of 50ms. The ACS does not provide any position. IGRACS bursts are emitted by gamma-ray bursts and other sources. The catalogue of IGRACS (including lightcurves) will be published electronically on http://www.isdc.unige.ch/integral/
Auth.:	Roland Walter INTEGRAL Science Dat Centre
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: IGRW
IGRW	(INTEGRAL WEAK trigger)
Write:	<<IGRW YYMMDD>>
N:	15
Object:	(Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	Swift follow-up observations of N=15 INTEGRAL WEAK triggers (below 8σ significance).
Ref:	=2017MNRAS.470..314H
by	HIGGINS A.B. , STARLING R.L.C., GOTZ D., MEREGHETTI S., WIERSEMA K., MACCARONE T., OSBORNE J.P., TANVIR N.R., O'BRIEN P.T., BIRD A.J., ROWLINSON A., GEHRELS N.
	Mon. Not. R. Astron. Soc., 470, 314-323 (2017)
	Investigating the nature of the INTEGRAL γ-ray bursts and sub-threshold triggers with Swift follow-up.
o	Table 1: <IGRW YYMMDD> N=15.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [IGS2002]
[IGS2002]	(Ivison+Greve+Smail+, 2002)= (SCUBA)
Write:	<<[IGS2002] LE 850.NN>> <<[IGS2002] N2 850.NN>> <<[IGS2002] LE 850.NNa>>
N:	21+15+5
Object:	(submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SCUBA survey at 850mu.m centered on two fields: Lockman Hole and ELAIS N2. Search for radio counterparts in LE 850.8 and LE 850.14: 3 sources 8a to 8c, 2 sources 14a and 14b. (Nos 1-21) in Lockman Hole and (Nos 1-15) in ELAIS N2 fields are equivalent to [SFD2002] LHE NN and [SFD2002] N2 NN. See also [SFD2002] and [MSD2005].
in source:	NAME Lockman Hole
in source:	ELAIS N2
Ref:	=2002MNRAS.337....1I
by	IVISON R.J. , GREVE T.R., SMAIL I., DUNLOP J.S., ROCHE N.D., SCOTT S.E., PAGE M.J., STEVENS J.A., ALMAINI O., BLAIN A.W., WILLOTT C.J., FOX M.J., GILBANK D.G., SERJEANT S., HUGHES D.H.
	Mon. Not. R. Astron. Soc., 337, 1-25 (2002)
	Deep radio imaging of the SCUBA 8-mJy survey fields: submillimetre source identifications and redshift distribution.
o	Table 1: <[IGS2002] LE 850.NN> (Nos 1-21), <[IGS2002] N2 850.NN> (Nos 1-15).
Ref:	=2004ApJS..154..130E
by	EGAMI E. , DOLE H., HUANG J.-S., PEREZ-GONZALEZ P., LE FLOC'H E., PAPOVICH C., BARMBY P., IVISON R.J., SERJEANT S., MORTIER A., FRAYER D.T., RIGOPOULOU D., LAGACHE G., RIEKE G.H., WILLNER S.P., ALONSO-HERRERO A., BAI L., ENGELBRACHT C.W., FAZIO G.G., GORDON K.D., HINES D.C., MISSELT K.A., MIYAZAKI S., MORRISON J.E., RIEKE M.J., RIGBY J.R., WILSON G.
	Astrophys. J., Suppl. Ser., 154, 130-136 (2004)
	Spitzer observations of the SCUBA/VLA sources in the Lockman hole: star formation history of infrared-luminous galaxies.
o	Fig.2, Table 1: <[IGS2002] LE 850.NNa> (Nos 8a to 8c, 14a, 14b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IGS2004]
[IGS2004]	(Ivison+Greve+Serjeant+, 2004)
Write:	<<[IGS2004] MM JHHMMSS.s+DDMMSS>>
N:	9
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spitzer Early Release observations of 9 luminous, dusty galaxies selected by MAMBO on the IRAM 30m telescope. See also [GIB2004].
Ref:	=2004ApJS..154..124I
by	IVISON R.J. , GREVE T.R., SERJEANT S., BERTOLDI F., EGAMI E., MORTIER A.M.J., ALONSO-HERRERO A., BARMBY P., BEI L., DOLE H., ENGELBRACHT C.W., FAZIO G.G., FRAYER D.T., GORDON K.D., HINES D.C., HUANG J.-S., LE FLOC'H E., MISSELT K.A., MIYAZAKI S., MORRISON J.E., PAPOVICH C., PEREZ-GONZALEZ P.G., RIEKE M.J., RIEKE G.H., RIGBY J., RIGOPOULOU D., SMAIL I., WILSON G., WILLNER S.P.
	Astrophys. J., Suppl. Ser., 154, 124-129 (2004)
	Spitzer observations of MAMBO galaxies: weeding out active nuclei in starbursting protoellipticals.
o	Table 1: <[IGS2004] MM JHHMMSS.s+DDMMSS> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IGVV
IGVV	(Interacting G, Vorontsov-Vel'yaminov)
*****	Avoid the usage of IGVV, prefer VV
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Ih
Ih	(Ikhsanov)
*****	Avoid the usage of Ih, prefer [I59]
Origin	of the Acronym: L (1959PAZh...23..458Z)
Details on Acronym: IH-alpha
IH-alpha	(Institute in Hawaii, H-alpha obj.)
*****	Avoid the usage of IH-alpha, prefer IfAHA
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [IHA2007]
[IHA2007]	(Irwin+Hodgkin+Aigrain+, 2007)
Write:	<<[IHA2007] N2516-N-N-NNNN>>
N:	362
Object:	* (SIMBAD class: Star)
Note:	CTIO 4m Blanco telescope photometry of the young cluster NGC 2516.
in source:	NGC 2516
Ref:	=2007MNRAS.377..741I
by	IRWIN J. , HODGKIN S., AIGRAIN S., HEBB L., BOUVIER J., CLARKE C., MORAUX E., BRAMICH D.M.
	Mon. Not. R. Astron. Soc., 377, 741-758 (2007)
	The Monitor project: rotation of low-mass stars in the open cluster NGC2516.
o	Table 1: <[IHA2007] N2516-N-N-NNNN> N=362.
=E=	Catalogue in electronic form as J/MNRAS/377/741
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IHA2008]
[IHA2008]	(Irwin+Hodgkin+Aigrain+, 2008)= ([IHA2008a])
Write:	<<[IHA2008] N2547-N-N-NNNN>>
N:	176
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	MPG-ESO 2.2m telescope WFI survey of NGC 2547.
in source:	NGC 2547
Ref:	=2008MNRAS.383.1588I
by	IRWIN J. , HODGKIN S., AIGRAIN S., BOUVIER J., HEBB L., MORAUX E.
	Mon. Not. R. Astron. Soc., 383, 1588-1602 (2008)
	The Monitor project: rotation of low-mass stars in the open cluster NGC 2547.
o	Table 1: <[IHA2008] N2547-N-N-NNNN> N=176.
=E=	Catalogue in electronic form as J/MNRAS/383/1588
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IHA2008a]
[IHA2008a]	(Irwin+Hodgkin+Aigrain+, 2008)
*****	Avoid the usage of [IHA2008a], prefer [IHA2008]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IHA2008b]
[IHA2008b]	(Irwin+Hodgkin+Aigrain+, 2008)
Write:	<<[IHA2008b] N2362-N-NNNNN>>
N:	271
Object:	* in Cl* (SIMBAD class: Star)
Note:	CTIO 4m Blanco telescope and Mosaic-II detector observations as part of the Monitor project. Search for rotating low-mass stars.
in source:	NGC 2362
Ref:	=2008MNRAS.384..675I
by	IRWIN J. , HODGKIN S., AIGRAIN S., BOUVIER J., HEBB L., IRWIN M., MORAUX E.
	Mon. Not. R. Astron. Soc., 384, 675-686 (2008)
	The Monitor project: rotation of low-mass stars in NGC 2362 - testing the disc regulation paradigm at 5 Myr.
o	Table 1: <[IHA2008b] N2362-N-NNNNN> N=271.
=E=	Catalogue in electronic form as J/MNRAS/384/675
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IHC2016]
[IHC2016]	(Ishigaki+Hwang+Chiba+, 2016)
Write:	<<[IHC2016] CEN sNN>> <<[IHC2016] FDNN NN>>
N:	19+130
Object:	* (SIMBAD class: Star)
Note:	Subaru FOCAS and Keck DEIMOS spectroscopic observations of the field of Cl Pal 5.
in source:	Cl Pal 5
Ref:	=2016ApJ...823..157I
by	ISHIGAKI M.N. , HWANG N., CHIBA M., AOKI W.
	Astrophys. J., 823, 157 (2016)
	Line-of-sight velocity and metallicity measurements of the Palomar 5 tidal stream.
o	Table 4: <[IHC2016] CE1 sNN> N=9 among (Nos s1-s21), <[IHC2016] CE2 sNN> N=10 among (Nos s8-s24). Table 5: <[IHC2016] FDNN NN> N=130 among (Nos FD1-2 to FD10 80).
=E=	Catalogue in electronic form as J/ApJ/823/157
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IHD2003]
[IHD2003]	(Imai+Horiuchi+Deguchi+, 2003) (Not yet in Simbad)
Write:	<<[IHD2003] NN>>
N:	61
Object:	H2O Maser feature (SIMBAD class: Maser)
Note:	See also [IKS2000].
in source:	[WBN72] W 3 IRS 5
Ref:	=2003ApJ...595..285I
by	IMAI H. , HORIUCHI S., DEGUCHI S., KAMEYA O.
	Astrophys. J., 595, 285-293 (2003)
	Linear polarization observations of water masers in W3 IRS 5.
o	Table 1: <[IHD2003] NN> (Nos 1-61).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IHS2009]
[IHS2009]	(Irwin+Hoffman+Spekkens, 2009+)
Write:	<<[IHS2009] N2903-HI-1>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Note:	Arecibo/Arecibo L-band Feed Array (ALFA) HI survey of NGC 2903.
Ref:	=2009ApJ...692.1447I
by	IRWIN J.A. , HOFFMAN G.L., SPEKKENS K., HAYNES M.P., GIOVANELLI R., LINDER S.M., CATINELLA B., MOMJIAN E., KORIBALSKI B.S., DAVIES J., BRINKS E., DE BLOK W.J.G., PUTMAN M.E., VAN DRIEL W.
	Astrophys. J., 692, 1447-1463 (2009)
	ΛCDM satellites and H I companions–the Arecibo ALFA survey of NGC 2903.
o	J080538+210651, J093215+211243, J102155+215931 are not identified because of an incomplete format.
o	Text, Table 6: <[IHS2009] N2903-HI-1>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: II
II	(Roman num. list II)
*****	Avoid the usage of II, prefer IC
Details on Acronym: II
II	(Iijima+Ishida)
*****	Avoid the usage of II, prefer [II78]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [II78]
[II78]	(Iijima+Ishida, 1978)= (II)
Write:	<<[II78] NN>> <<[II78] NN-N>>
N:	56
Object:	* (SIMBAD class: Star)
Note:	(Nos 1-55), Nos 39-1 and 39-2
Ref:	=1978PASJ...30..657I
by	IIJIMA T. , ISHIDA K.
	Publ. Astron. Soc. Jap., 30, 657-670 (1978)
	Two-micron objects in the northern Monoceros region.
o	<[II78] NN> <[II78] NN-N> N=56
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IIB2000]
[IIB2000]	(Ibata+Irwin+Bienayme+, 2000)
Write:	<<[IIB2000] FNNN-NN>>
N:	2
Object:	PM* (SIMBAD class: HighPM* = High Proper Motion Star)
Note:	Discovery of N=2 VHPM (Very High Proper Motion) stars.
Ref:	=2000ApJ...532L..41I
by	IBATA R. , IRWIN M., BIENAYME O., SCHOLZ R., GUIBERT J.
	Astrophys. J., 532, 41-45 (2000)
	Discovery of high proper-motion ancient white dwarfs: nearby massive compact halo objects?.
o	<[IIB2000] FNNN-NN> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IIB2009]
[IIB2009]	(Ibar+Ivison +Biggs+, 2009)= (LH610MHz) = (LH1.4GHz) = ([IIB2009a])
Write:	<<[IIB2009] LH610MHz JHHMMSS.s+DDMMSSa>> <<[IIB2009] LH1.4GHz JHHMMSS.s+DDMMSSa>>
N:	1587+1452
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	GMRT (610MHz) and VLA (1.4GHz) observations of the Lockman Hole.
in source:	NAME Lockman Hole
Ref:	=2009MNRAS.397..281I
by	IBAR E. , IVISON R.J., BIGGS A.D., LAL D.V., BEST P.N., GREEN D.A.
	Mon. Not. R. Astron. Soc., 397, 281-298 (2009)
	Deep multi-frequency radio imaging in the Lockman Hole using the GMRT and VLA - I. The nature of the sub-mJy radio population.
o	Table 3: <[IIB2009] LH610MHz JHHMMSS.s+DDMMSSa> N=1587. Table 4: <[IIB2009] LH1.4GHz JHHMMSS.s+DDMMSSa> N=1452.
=E=	Catalogue in electronic form as J/MNRAS/397/281
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [III2004]
[III2004]	(Ishikawa+Ishida+Ishisaki+, 2004)
Write:	<<[III2004] M 4 NN>> <<[III2004] NGC 6397 N>>
N:	14+8
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ASCA observations of M 4 and NGC 6397 globular clusters. Only the cores of the globular clusters are detected.
in source:	M 4 = NGC 6121
in source:	NGC 6397
Ref:	=2004PASJ...56..453I
by	ISHIKAWA T. , ISHIDA M., ISHISAKI Y., OHASHI T., YAMASAKI N.Y.
	Publ. Astron. Soc. Jap., 56, 453-464 (2004)
	ASCA observations of the two nearest globular clusters, M 4 and NGC 6397.
o	Table 3: XN = [JVH94] NGC NNNN N
o	Table 3: <[III2004] M 4 NN> (Nos 1-14), <[III2004] NGC 6397 N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IIL98]
[IIL98]	(Irwin+Ibata+Lewis+, 1998)
Write:	<<[IIL98] QSO J0831+5245 abs N.NN>>
N:	3
Object:	Absorber
Note:	N=3 absorption systems in the line of sight of the QSO NAME APM 08279+5255 = QSO J0831+5245 See also [PAS2000], [EIP2004].
Ref:	=1998ApJ...505..529I
by	IRWIN M.J. , IBATA R.A., LEWIS G.F., TOTTEN E.J.
	Astrophys. J., 505, 529-535 (1998)
	APM 08279+5255: an ultraluminous broad absorption line quasar at a redshift z = 3.87.
o	Fig.1: <[IIL98] QSO J0831+5245 abs N.NN> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IIM2000]
[IIM2000]	(Iye+Iwamuro+Maihara+, 2000)
Write:	<<[IIM2000] RN>>
N:	5
Object:	Extremely Red Obj. (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Subaru observations. N=5 identified Extremely Red Objects (ERO) in ACO 851.
in source:	ACO 851 = ClG 0939+4713
Ref:	=2000PASJ...52....9I
by	IYE M. , IWAMURO F., MAIHARA T., MIYAZAKI S., OKAMURA S., SHIMASAKU K., SIMPSON C., AKIYAMA M., ANDO H., AOKI T., AOKI T., CHIKADA Y., DOI M., EBIZUKA N., FUKUDA T., FURUSAWA H., GOTO M., HAMABE M., HATA R., HAYASHI M., HAYASHI S.S., HORAGUCHI T., ICHIKAWA S., ICHIKAWA T., IMANISHI M., IMI K., INATA M., ISOBE S., ITOH Y., IWAI J., KAIFU N., KAMATA Y., KANZAWA T., KAROJI H., KASHIKAWA N., KATO T., KAWASAKI W., KIMURA M., KOBAYASHI N., KOBAYASHI Y., KODAIRA K., KOMIYAMA Y., KOSUGI G., KURAKAMI T., MIKAMI Y., MIYASHITA A., MIYATA T., MIZUMOTO Y., MOTOHARA K., NAKAGIRI M., NAKAJIMA K., NAKAMURA K., NAKATA F., NARIAI K., NISHIHARA E., NISHIKAWA J., NISHIMURA S., NISHIMURA T., NISHINO T., NOGUCHI K., NOGUCHI T., NOUMARU J., OGASAWARA R., OKADA N., OKITA K., OMATA K., OSHIMA N., OTSUBO M., OYA S., SASAKI G., SASAKI T., SAWADA Y., SEKIGUCHI K., SEKIGUCHI M., SHELTON I., SUTO H., SUZUKI K., TAGUCHI T., TAKAMI H., TAKATA T., TAKATO N., TAMURA M., TANABE H., TANAKA K., TANAKA W., TERADA H., TOMONO D., TORII Y., TSUKAMOTO H., USUDA T., WATANABE J., WATANABE M., YAGI M., YAMASHITA T., YAMASHITA Y., YASUDA N., YOSHIDA M., YOSHIDA S., YUTANI M.
	Publ. Astron. Soc. Jap., 52, 9-23 (2000)
	Subaru first-light deep photometry of galaxies in A 851 field.
o	Table 2: <[IIM2000] RN> (Nos R1-R5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IIM2019]
[IIM2019]	(Iwata+Inoue+Micheva+, 2019)
Write:	<<[IIM2019] LAENNN>>
N:	8
Object:	LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Subaru SuprimeCam narrow-band imaging and MOIRCS spectroscopy of N=5+3 Lyman α emitters (LAEs).
in source:	NAME GOODS North Field
Ref:	=2019MNRAS.488.5671I
by	IWATA I. , INOUE A.K., MICHEVA G., MATSUDA Y., YAMADA T.
	Mon. Not. R. Astron. Soc., 488, 5671-5689 (2019)
	Subaru narrow-band imaging search for Lyman continuum from galaxies at z > 3 in the GOODS-N field.
o	Tables 3+5: <[IIM2019] LAENNN> N=8 among (Nos LAE019-LAE137).
o	Identifications in Simbad: R06 = [RSE2006] ; MOSDEF NNNNN = [SWM2014] GOODS-N NNNNN ; S03-MNN = SAS-LBG HDF-MNN ; B02-NNN = [BAH2001] NNN ; FMMSSs-MMSS = [DSB2001] FMMSSs-MMSS ; hdN-xxxx-yyyy = [LKG97] hdN-xxxx-yyyy.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IJC2004]
[IJC2004]	(Indebetouw+Johnson+Conti, 2004)
Write:	<<[IJC2004] BHHMM+DDMM>> <<[IJC2004] BHHMM+DDMM(W)>> <<[IJC2004] BHHMM+DDMM(WN)>> <<[IJC2004] BHHMM+DDMM(WW)>> <<[IJC2004] BHHMM+DDMM(WWN)>> <<[IJC2004] BHHMM+DDMM(N)>>
N:	13+58
Object:	*(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA observations of the Magellanic Clouds. N=13 compact sources in [FJW97] sources in the SMC, and N=58 compact sources in [FHW95] sources in the LMC.
in source:	Magellanic Clouds:LMC = LMC
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2004AJ....128.2206I
by	INDEBETOUW R. , JOHNSON K.E., CONTI P.
	Astron. J., 128, 2206-2233 (2004)
	Australia telescope compact array survey of candidate ultracompact and buried H II regions in the Magellanic Clouds.
o	Table 4 : B0522-5800 is a misprint for -6800 (= [FHW95] LMC B0522-6800)
o	Tables 3, 4: <[IJC2004] BHHMM+DDMM>, <[IJC2004] BHHMM+DDMM(W)>, <[IJC2004] BHHMM+DDMM(WN)>, <[IJC2004] BHHMM+DDMM(WW)>, <[IJC2004] BHHMM+DDMM(WWN)>, <[IJC2004] BHHMM+DDMM(N)>, N=13+58.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IK
IK	(Israel+van der Kruit)
*****	Avoid the usage of IK, prefer [IV74]
Origin	of the Acronym: L (1978A&A....62...51V)
Details on Acronym: [IK2011]
[IK2011]	(Ikeda+Kitamura, 2011)
Write:	<<[IK2011] NNN>>
N:	123
Object:	C18O Core (SIMBAD class: denseCore = Dense Core)
Note:	Nobeyama 45m telescope C18O(1-0) observations of molecular gas associated with Sh 2-140.
in source:	SH 2-140
Ref:	=2011ApJ...732..101I
by	IKEDA N. , KITAMURA Y.
	Astrophys. J., 732, 101 (2011)
	Similarity between the C^{18}O (J = 1-0) core mass function and the initial mass function (IMF) in the S140 region.
o	Table 1: <[IK2011] NNN> (Nos 1-123).
=E=	Catalogue in electronic form as J/ApJ/732/101
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IKA2000]
[IKA2000]	(In'T Zand+Kuiper+Amati+, 2000)
Write:	<<[IKA2000] SN>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	BeppoSAX observations of GRB 991014. N=2 X-ray sources in the field of GRB 991014.
Ref:	=2000ApJ...545..266I
by	IN'T ZAND J.J.M. , KUIPER L., AMATI L., ANTONELLI L.A., HURLEY K., COLETTA A., COSTA E., FEROCI M., FRONTERA F., GANDOLFI G., HEISE J., KUULKERS E., MULLER J.M., NICASTRO L., PIRO L., SMITH M.J.S., TAVANI M.
	Astrophys. J., 545, 266-270 (2000)
	X-ray afterglow detection of the short γ-ray burst GRB 991014.
o	<[IKA2000] SN> (Nos S1-S2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IKA2001]
[IKA2001]	(In't Zand+Kuiper+Amati+, 2001)
Write:	<<[IKA2001] JHHMMSS.s+DDMMSS.s>>
N:	3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	BeppoSAX observations of the field of GRB 010222. N=3 X-ray sources.
Ref:	=2001ApJ...559..710I
by	IN'T ZAND J.J.M. , KUIPER L., AMATI L., ANTONELLI L.A., BUTLER R.C., COSTA E., FEROCI M., FRONTERA F., GANDOLFI G., GUIDORZI C., HEISE J., KAPTEIN R.G., KUULKERS E., NICASTRO L., PIRO L., SOFFITTA P., TAVANI M.
	Astrophys. J., 559, 710-715 (2001)
	BeppoSAX measurements of the bright γ-ray burst 010222.
o	Fig.3, text: <[IKA2001] JHHMMSS.s+DDMMSS.s> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IKA2011]
[IKA2011]	(Ikarashi+Kohno+Aguirre+, 2011)
Write:	<<[IKA2011] SXDF1100.001>>
N:	1
Object:	Submm G (SIMBAD class: Galaxy)
Note:	ASTE AzTEC 1100µm observations of N=1 submillimeter galaxy in the Subaru/XMM-Newton Deep Field.
in source:	NAME SXDF
Ref:	=2011MNRAS.415.3081I
by	IKARASHI S. , KOHNO K., AGUIRRE J.E., ARETXAGA I., ARUMUGAM V., AUSTERMANN J.E., BOCK J.J., BRADFORD C.M., CIRASUOLO M., EARLE L., EZAWA H., FURUSAWA H., FURUSAWA J., GLENN J., HATSUKADE B., HUGHES D.H., IONO D., IVISON R.J., JOHNSON S., KAMENETZKY J., KAWABE R., LUPU R., MALONEY P., MATSUHARA H., MAUSKOPF P.D., MOTOHARA K., MURPHY E.J., NAKAJIMA K., NAKANISHI K., NAYLOR B.J., NGUYEN H.T., PERERA T.A., SCOTT K.S., SHIMASAKU K., TAKAGI T., TAKATA T., TAMURA Y., TANAKA K., TSUKAGOSHI T., WILNER D.J., WILSON G.W., YUN M.S., ZMUIDZINAS J.
	Mon. Not. R. Astron. Soc., 415, 3081-3096 (2011)
	Detection of an ultrabright submillimetre galaxy in the Subaru/XMM–Newton deep field using AzTEC/ASTE.
o	<[IKA2011] SXDF1100.001> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IKE2013]
[IKE2013]	(Irwin+Krause+English+, 2013)
Write:	<<[IKE2013] CHANG-ES A>> <<[IKE2013] N>>
N:	2+7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	JVLA observations at 1.5 and 6GHz of UGC 10288, as part of the Continuum Halos in Nearby Galaxies - an EVLA Survey (CHANG-ES).
in source:	UGC 10288
Ref:	=2013AJ....146..164I
by	IRWIN J. , KRAUSE M., ENGLISH J., BECK R., MURPHY E., WIEGERT T., HEALD G., WALTERBOS R., RAND R.J., PORTER T.
	Astron. J., 146, 164 (2013)
	CHANG-ES. III. UGC 10288 - An edge-on galaxy with a background double-lobed radio source.
o	p.16: UGC 1028 is a misprint for UGC 10288.
o	Paragr. 3.1: <[IKE2013] CHANG-ES A> (Nos A-B). Fig. 6, Table 6: <[IKE2013] N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IKI2011]
[IKI2011]	(Inoue+Kousai+Iwata+, 2011)
Write:	<<[IKI2011] a>>
N:	9
Object:	LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT VIMOS and Subaru FOCAS observations of N=9 LAEs.
in source:	SSA 22
Ref:	=2011MNRAS.411.2336I
by	INOUE A.K. , KOUSAI K., IWATA I., MATSUDA Y., NAKAMURA E., HORIE M., HAYASHINO T., TAPKEN C., AKIYAMA M., NOLL S., YAMADA T., BURGARELLA D., NAKAMURA Y.
	Mon. Not. R. Astron. Soc., 411, 2336-2352 (2011)
	Lyman `bump' galaxies – II. A possible signature of massive extremely metal-poor or metal-free stars in z= 3.1 Lyα emitters.
o	Table 1, Fig. 1: <[IKI2011] a> (Nos a-i).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IKO2015]
[IKO2015]	(Ishigaki+Kawamata+Ouchi+, 2015)
Write:	<<[IKO2015] {HFF1}{C\|P}-{i\|Y}NN>> <<[IKO2015] {HFF1}{C\|P}-{YJ}N>> <<[IKO2015] NN.N>>
N:	35+15+6+67
Object:	G + Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST (ACS and WFC3) observations of the galaxy cluster Abell 2744, as part of the Hubble Frontier Fields program. N=35 i-dropout candidates at z∼6-7, N=15 Y-dropout candidates at z∼8, N=6 Y J-dropout candidates at z∼9 and N=67 images of 24 multiply imaged systems were detected. See also [ARK2014], [ARK2015], [ZSM2014], [ZZB2014], [RJL2014], [MCD2011] and [LBD2014].
in source:	ACO 2744
Ref:	=2015ApJ...799...12I
by	ISHIGAKI M. , KAWAMATA R., OUCHI M., OGURI M., SHIMASAKU K., ONO Y.
	Astrophys. J., 799, 12 (2015)
	Hubble frontier fields first complete cluster data: faint galaxies at z ~ 5-10 for UV luminosity functions and cosmic reionization.
o	Table 2: <[IKO2015] HFF1C-iNN> (Nos i1-i18), <[IKO2015] HFF1P-iNN> (Nos i1-i17). Table 3: <[IKO2015] HFF1C-YNN> (Nos Y1-Y11), <[IKO2015] HFF1P-YN> (Nos Y1-Y4). Table 4: <[IKO2015] HFF1C-YJ1>, <[IKO2015] HFF1P-YJN> (Nos YJ1-YJ3). Table 6: <[IKO2015] NN.N> (Nos 1.1-1.3 to 24.1-24.2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IKO2018]
[IKO2018]	(Ishigaki+Kawamata+Ouchi+, 2018)
Write:	<<[IKO2018] HFFNA-SSss-MSSs>>
N:	350+60+40
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST ACS and WFC3 observations of N=350+66+40 drop-out galaxy candidates at z∼6-7, 8, and 9, respectively, in the six Hubble Frontier Fields and the six parallel fields. The letter "A" in the format stands for C or P, and indicates whether a source is in a cluster field or a parallel field. The second part of the format shows the last four digits of right ascension and declination SSss-MSSs. Use of all of cluster and parallel fields data taken by the Hubble Frontier Fields (HFF) program.
in source:	ACO 2744
in source:	MCS J0416.1-2403
in source:	ClG J0717+3745 = MCS J0717.5+3745
in source:	ClG J1149+2223 = MCS J1149.5+2223
in source:	RXC J2248.7-4431 = ACO S 1063
in source:	ACO 370
Ref:	=2018ApJ...854...73I
by	ISHIGAKI M. , KAWAMATA R., OUCHI M., OGURI M., SHIMASAKU K., ONO Y.
	Astrophys. J., 854, 73-73 (2018)
	Full-data results of Hubble Frontier Fields: UV luminosity functions at z ~ 6-10 and a consistent picture of cosmic reionization.
o	Tables 4-6: <[IKO2018] HFFNA-SSss-MSSs> N=350+60+40.
=E=	Catalogue in electronic form as <J/ApJ/854/73/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IKP2016]
[IKP2016]	(Immer+Kauffmann+Pillai+, 2016)
Write:	<<[IKP2016] NN km s-1 cloud>> <<[IKP2016] GLL.lll+B.bbb>>
N:	5
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	APEX H2CO line observations of N=5 molecular clouds in the central molecular zone (CMZ). Use of the APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) at 218 and 291 GHz.
in source:	NAME Galactic Center
Ref:	=2016A&A...595A..94I
by	IMMER K. , KAUFFMANN J., PILLAI T., GINSBURG A., MENTEN K.M.
	Astron. Astrophys., 595A, 94-94 (2016)
	Temperature structures in Galactic center clouds. Direct evidence for gas heating via turbulence.
o	Table 1: <[IKP2016] NN km s-1 cloud> (Nos 20, 50), <[IKP2016] GLL.lll+B.bbb> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IKPM
IKPM	(Irwin+Kennedy+Parkin+Madden)
Write:	<<IKPM N>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	SDSS DR5 data of NGC 5529. N=2 new companions are found.
Ref:	=2007A&A...474..461I
by	IRWIN J.A. , KENNEDY H., PARKIN T., MADDEN S.
	Astron. Astrophys., 474, 461-472 (2007)
	PAHs in the halo of NGC 5529.
o	Kregel B is [KVD2004] NGC 5529 B
o	Fig.1, Table 2: <IKPM N> (Nos 1-2).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [IKS2000]
[IKS2000]	(Imai+Kameya+Sasao+, 2000)= (I2000) (Not yet in Simbad)
Write:	<<[IKS2000] NNN>>
N:	108
Object:	H2O Maser (SIMBAD class: Maser)
Note:	N=108 H2O maser features etected towards [WBN72] W 3 IRS 5. See also [IHD2003].
in source:	[WBN72] W 3 IRS 5
Ref:	=2000ApJ...538..751I
by	IMAI H. , KAMEYA O., SASAO T., MIYOSHI M., DEGUCHI S., HORIUCHI S., ASAKI Y.
	Astrophys. J., 538, 751-765 (2000)
	Kinematics and distance of water masers in W3 IRS 5.
o	Table 3: <[IKS2000] NNN> (Nos 1-108).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IKS2009]
[IKS2009]	(Ikeda+Kitamura+Sunada, 2009)
Write:	<<[IKS2009] H13CO+ NNN>> <<[IKS2009] SMM JHHMMmm+DDMMm>>
N:	151+82
Object:	Core (SIMBAD class: PartofCloud = Part of Cloud)
Note:	Nobeyama 45m radio telescope observations of Ori B Cloud. N=151 H13CO+ dense cores. N=82 850mu.m cores: see also [JFM2001] and [JMM2006].
in source:	NAME Ori B
Ref:	=2009ApJ...691.1560I
by	IKEDA N. , KITAMURA Y., SUNADA K.
	Astrophys. J., 691, 1560-1582 (2009)
	A survey of dense cores in the Orion B cloud.
o	Table 1: <[IKS2009] H13CO+ NNN> (Nos 1-151). Table 4: <[IKS2009] SMM JHHMMmm+DDMMm> N=82.
=E=	Catalogue in electronic form as <J/ApJ/691/1560/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IKT
IKT	(Inoue+Koyama+Tanaka)
Write:	<<IKT NN>>
N:	25
Object:	(Soft X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Einstein IPC observations. Association with Neb. or Radio SNR
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1983IAUS..101..535I
by	INOUE H. , KOYAMA K., TANAKA Y.
	IAU Symp., 101, held in Venice, Italy, 30 Aug - 02 Sep 1982, Ed. John Danziger and Paul Gorenstein: Supernova Remnants and their X-ray emission, 101, 535-540 (1983)
	Soft X-ray observation of Supernova Remnants in the Small Magellanic Cloud.
o	Table I: <IKT NN> (Nos 1-25)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: IKT
IKT	(Imanishi+Koyama+Tsuboi)
*****	Avoid the usage of IKT, prefer [IKT2001]
Origin	of the Acronym: L (2003PASJ...55..653I)
Details on Acronym: [IKT2001]
[IKT2001]	(Imanishi+Koyama+Tsuboi, 2001)= (IKT) = (ROXCH)
Write:	<<[IKT2001] NN>>
N:	87
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-I observations of rho Oph cloud. See also [INT2003].
in source:	NAME rho Oph Cloud
Ref:	=2001ApJ...557..747I
by	IMANISHI K. , KOYAMA K., TSUBOI Y.
	Astrophys. J., 557, 747-760 (2001)
	Chandra observation of the ρ Ophiuchi cloud.
o	(Erratum) erratum vol. 579, p. 920 (2002)
o	Table 1: <[IKT2001] NN> (Nos 1-87).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ILB98]
[ILB98]	(Ibata+Lewis+Beaulieu, 1998)
Write:	<<[ILB98] JHHMMSS.s+DDMMSS.ss>>
N:	40
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	'VRC' (Vertical Red Clump) population in the LMC
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1998ApJ...509L..29I
by	IBATA R.A. , LEWIS G.F., BEAULIEU J.-P.
	Astrophys. J., 509, 29-32 (1998)
	Reexamination of the possible tidal stream in front of the Large Magellanic Cloud.
o	Table 1: <[ILB98] JHHMMSS.s-DDMMSS.ss> N=40.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ILC2007]
[ILC2007]	(Im+Lee+Cho+, 2007)
Write:	<<[ILC2007] NN>>
N:	40
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	Discovery of 40 bright QSOs near the Galactic Plane from the SNUQSO survey.
Ref:	=2007ApJ...664...64I
by	IM M. , LEE I., CHO Y., CHOI C., KO J., SONG M.
	Astrophys. J., 664, 64-70 (2007)
	Seoul national university bright quasar survey in optical (SNUQSO). II. Discovery of 40 bright quasars near the Galactic plane.
o	Table 1, col(1): <[ILC2007] NN> (Nos 1-40) = Table 1, col(2): <SNUQSO JHHMMSS.ss+DDMMSS.s> N=40.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ILF-1
ILF-1	(Intermediate Latitude, Field 1)
*****	Avoid the usage of ILF-1, prefer ILF1
Origin	of the Acronym: L = Found in the literature
Details on Acronym: ILF1
ILF1	(Intermediate Latitude, Field 1)= (ILF-1) = (MacRae)
Write:	<<ILF1 +DD NNN>>
N:	939
Object:	* (SIMBAD class: Star)
Ref:	=1952ApJ...116..592M
by	MacRAE D.A.
	Astrophys. J., 116, 592-611 (1952)
	Stellar spectra and colors in Cygnus at galactic latitude +14 °.
o	<ILF1 +DD NNN> N=939
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [ILI99]
[ILI99]	(Ibata+Lewis+Irwin+, 1999)
Write:	<<[ILI99] APM 08279+5255 A>>
N:	3
Object:	Lensing image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Stat:	is completely incorporated in Simbad
Note:	HST NICMOS observations. N=3 lensed images of the QSO APM 08279+5255.
in source:	NAME APM 08279+5255
Ref:	=1999AJ....118.1922I
by	IBATA R.A. , LEWIS G.F., IRWIN M.J., LEHAR J., TOTTEN E.J.
	Astron. J., 118, 1922-1930 (1999)
	NICMOS and VLA observations of the gravitationally lensed ultraluminous BAL quasar APM 08279+5255: detection of a third image.
o	<[ILI99] APM 08279+5255 A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ILL2017]
[ILL2017]	(Imara+Lada+Lewis+, 2017)
Write:	<<[ILL2017] Cal-X>> <<[ILL2017] A>> <<[ILL2017] California-X>> (not recognised by Simbad, but found in literature)
N:	1+8
Object:	Part of Cloud + Core (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HHT 12CO and 13CO observations of N=1 X-shaped region in the California molecular cloud, and N=8 cores in this region. Use of Auriga-California Molecular Cloud (ACMC) Herschel data.
in source:	NAME California Molecular Cloud
Ref:	=2017ApJ...840..119I
by	IMARA N. , LADA C., LEWIS J., BIEGING J.H., KONG S., LOMBARDI M., ALVES J.
	Astrophys. J., 840, 119-119 (2017)
	X marks the spot: nexus of filaments, cores, and outflows in a young star-forming region.
o	<[ILL2017] Cal-X> N=1. Fig. 8, Table 3: <[ILL2017] A> (Nos A-H).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ILS
ILS	(Intermediate Latitude Service)= (MD) (Not yet in Simbad)
Write:	<<ILS NNN>>
N:	440
Object:	* (SIMBAD class: Star)
Ref:	=1973CoORB..74....1M
by	MELCHIOR P. , DEJAIFFE R.
	Com. de l'Observ. Royal de Belgique, 74, 1-None (1973)
	Calcul des declinaisons et mouvements propres des etoiles du Service International des Latitudes a partir des catalogues meridiens.
o	1973: Ser. B. First published in 1969 Ann. Obs. R. Belgique, 3e ser., 10, 63-339.
o	<ILS NNN> (Nos 1-440).
Details on Acronym: ILT
ILT	(International LOFAR Telescope)
Write:	<<ILT JHHMMSS.s+DDMMSS.s>> <<ILT JHHMMSS.ss+DDMMSS.s>>
N:	44500+325694+4396228
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	LOFAR HBA (120-168MHz) observations as part of the LOFAR Two-metre Sky Survey (LoTSS). 2017A&A...598A.104S: Preliminary release (N=44500) 2019A&A...622A...1S: Data Release 1 (N=325694) 2022A&A...659A...1S: Data Release 2 (N=4396228) For more information, visit: https://lofar-surveys.org/
Ref:	=2017A&A...598A.104S
by	SHIMWELL T.W. , ROTTGERING H.J.A., BEST P.N., WILLIAMS W.L., DIJKEMA T.J., DE GASPERIN F., HARDCASTLE M.J., HEALD G.H., HOANG D.N., HORNEFFER A., INTEMA H., MAHONY E.K., MANDAL S., MECHEV A.P., MORABITO L., OONK J.B.R., RAFFERTY D., RETANA-MONTENEGRO E., SABATER J., TASSE C., VAN WEEREN R.J., BRUGGEN M., BRUNETTI G., CHYZY K.T., CONWAY J.E., HAVERKORN M., JACKSON N., JARVIS M.J., McKEAN J.P., MILEY G.K., MORGANTI R., WHITE G.J., WISE M.W., VAN BEMMEL I.M., BECK R., BRIENZA M., BONAFEDE A., CALISTRO RIVERA G., CASSANO R., CLARKE A.O., CSEH D., DELLER A., DRABENT A., VAN DRIEL W., ENGELS D., FALCKE H., FERRARI C., FROHLICH S., GARRETT M.A., HARWOOD J.J., HEESEN V., HOEFT M., HORELLOU C., ISRAEL F.P., KAPINSKA A.D., KUNERT-BAJRASZEWSKA M., McKAY D.J., MOHAN N.R., ORRU E., PIZZO R.F., PRANDONI I., SCHWARZ D.J., SHULEVSKI A., SIPIOR M., SMITH D.J.B., SRIDHAR S.S., STEINMETZ M., STROE A., VARENIUS E., VAN DER WERF P.P., ZENSUS J.A., ZWART J.T.L.
	Astron. Astrophys., 598A, 104-104 (2017)
	The LOFAR Two-metre Sky Survey. I. Survey description and preliminary data release.
o	<ILT JHHMMSS.s+DDMMSS.s> N=44500.
Ref:	=2019A&A...622A...1S
by	SHIMWELL T.W. , TASSE C., HARDCASTLE M.J., MECHEV A.P., WILLIAMS W.L., BEST P.N., ROTTGERING H.J.A., CALLINGHAM J.R., DIJKEMA T.J., DE GASPERIN F., HOANG D.N., HUGO B., MIRMONT M., OONK J.B.R., PRANDONI I., RAFFERTY D., SABATER J., SMIRNOV O., VAN WEEREN R.J., WHITE G.J., ATEMKENG M., BESTER L., BONNASSIEUX E., BRUGGEN M., BRUNETTI G., CHYZY K.T., COCHRANE R., CONWAY J.E., CROSTON J.H., DANEZI A., DUNCAN K., HAVERKORN M., HEALD G.H., IACOBELLI M., INTEMA H.T., JACKSON N., JAMROZY M., JARVIS M.J., LAKHOO R., MEVIUS M., MILEY G.K., MORABITO L., MORGANTI R., NISBET D., ORRU E., PERKINS S., PIZZO R.F., SCHRIJVERS C., SMITH D.J.B., VERMEULEN R., WISE M.W., ALEGRE L., BACON D.J., VAN BEMMEL I.M., BESWICK R.J., BONAFEDE A., BOTTEON A., BOURKE S., BRIENZA M., CALISTRO RIVERA G., CASSANO R., CLARKE A.O., CONSELICE C.J., DETTMAR R.J., DRABENT A., DUMBA C., EMIG K.L., ENSSLIN T.A., FERRARI C., GARRETT M.A., GENOVA-SANTOS R.T., GOYAL A., GURKAN G., HALE C., HARWOOD J.J., HEESEN V., HOEFT M., HORELLOU C., JACKSON C., KOKOTANEKOV G., KONDAPALLY R., KUNERT-BAJRASZEWSKA M., MAHATMA V., MAHONY E.K., MANDAL S., McKEAN J.P., MERLONI A., MINGO B., MISKOLCZI A., MOONEY S., NIKIEL-WROCZYNSKI B., O'SULLIVAN S.P., QUINN J., REICH W., ROSKOWINSKI C., ROWLINSON A., SAVINI F., SAXENA A., SCHWARZ D.J., SHULEVSKI A., SRIDHAR S.S., STACEY H.R., URQUHART S., VAN DER WIEL M.H.D., VARENIUS E., WEBSTER B., WILBER A.
	Astron. Astrophys., 622A, 1-1 (2019)
	The LOFAR Two-metre Sky Survey. II. First data release.
o	<ILT JHHMMSS.ss+DDMMSS.s> N=325694.
Ref:	=2022A&A...659A...1S
by	SHIMWELL T.W. , HARDCASTLE M.J., TASSE C., BEST P.N., ROTTGERING H.J.A., WILLIAMS W.L., BOTTEON A., DRABENT A., MECHEV A., SHULEVSKI A., VAN WEEREN R.J., BESTER L., BRUGGEN M., BRUNETTI G., CALLINGHAM J.R., CHYZY K.T., CONWAY J.E., DIJKEMA T.J., DUNCAN K., DE GASPERIN F., HALE C.L., HAVERKORN M., HUGO B., JACKSON N., MEVIUS M., MILEY G.K., MORABITO L.K., MORGANTI R., OFFRINGA A., OONK J.B.R., RAFFERTY D., SABATER J., SMITH D.J.B., SCHWARZ D.J., SMIRNOV O., O'SULLIVAN S.P., VEDANTHAM H., WHITE G.J., ALBERT J.G., ALEGRE L., ASABERE B., BACON D.J., BONAFEDE A., BONNASSIEUX E., BRIENZA M., BILICKI M., BONATO M., CALISTRO RIVERA G., CASSANO R., COCHRANE R., CROSTON J.H., CUCITI V., DALLACASA D., DANEZI A., DETTMAR R.J., DI GENNARO G., EDLER H.W., ENSSLIN T.A., EMIG K.L., FRANZEN T.M.O., GARCIA-VERGARA C., GRANGE Y.G., GURKAN G., HAJDUK M., HEALD G., HEESEN V., HOANG D.N., HOEFT M., HORELLOU C., IACOBELLI M., JAMROZY M., JELIC V., KONDAPALLY R., KUKRETI P., KUNERT-BAJRASZEWSKA M., MAGLIOCCHETTI M., MAHATMA V., MALEK K., MANDAL S., MASSARO F., MEYER-ZHAO Z., MINGO B., MOSTERT R.I.J., NAIR D.G., NAKONECZNY S.J., NIKIEL-WROCZYNSKI B., ORRU E., PAJDOSZ-SMIERCIAK U., PASINI T., PRANDONI I., VAN PIGGELEN H.E., RAJPUROHIT K., RETANA-MONTENEGRO E., RISELEY C.J., ROWLINSON A., SAXENA A., SCHRIJVERS C., SWEIJEN F., SIEWERT T.M., TIMMERMAN R., VACCARI M., VINK J., WEST J.L., WOLOWSKA A., ZHANG X., ZHENG J.
	Astron. Astrophys., 659A, 1-1 (2022)
	The LOFAR Two-metre Sky Survey. V. Second data release.
o	<ILT JHHMMSS.s+DDMMSS.s> N=4396228.
=E=	Catalogue in electronic form as <J/A+A/598/A104/>
=E=	Catalogue in electronic form as <J/A+A/622/A1/>
=E=	Catalogue in electronic form as <J/A+A/659/A1/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ILT2017]
[ILT2017]	(Ibata+Lewis+Thomas+, 2017)
Write:	<<[ILT2017] JHHMMSS.sss+DDMMSS.ss>>
N:	142
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT FLAMES and AAT AAOmega spectroscopy of N=154 stars in the Palomar 5 stellar stream.
in source:	NAME Palomar 5 Stream
Ref:	=2017ApJ...842..120I
by	IBATA R.A. , LEWIS G.F., THOMAS G., MARTIN N.F., CHAPMAN S.
	Astrophys. J., 842, 120-120 (2017)
	Feeling the pull: a study of natural galactic accelerometers. II. Kinematics and mass of the delicate stellar stream of the Palomar 5 globular cluster.
o	Table 2: <[ILT2017] JHHMMSS.sss+DDMMSS.ss> N=154.
=E=	Catalogue in electronic form as <J/ApJ/842/120/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ILW2016]
[ILW2016]	(Ivison+Lewis+Weiss+, 2016)
Write:	<<[ILW2016] GHH-NNNNNN>> <<[ILW2016] SGP-NNNNNN>> <<[ILW2016] NGP-NNNNNN>>
N:	47+33+32
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	N=47+33+32 dusty, star-forming galaxies selected from the Herschel-ATLAS survey. See also H-ATLAS. See also [VSE2016] (H-ATLAS DR1), [MVC2018] (H-ATLAS DRE).
Ref:	=2016ApJ...832...78I
by	IVISON R.J. , LEWIS A.J.R., WEISS A., ARUMUGAM V., SIMPSON J.M., HOLLAND W.S., MADDOX S., DUNNE L., VALIANTE E., VAN DER WERF P., OMONT A., DANNERBAUER H., SMAIL I., BERTOLDI F., BREMER M., BUSSMANN R.S., CAI Z.-Y., CLEMENTS D.L., COORAY A., DE ZOTTI G., EALES S.A., FULLER C., GONZALEZ-NUEVO J., IBAR E., NEGRELLO M., OTEO I., PEREZ-FOURNON I., RIECHERS D., STEVENS J.A., SWINBANK A.M., WARDLOW J.
	Astrophys. J., 832, 78-78 (2016)
	The space density of luminous dusty star-forming galaxies at z > 4: SCUBA-2 and LABOCA imaging of ultrared galaxies from Herschel-ATLAS.
o	Table 1, col(1): <H-ATLAS JHHMMSS.s+DDMMSS> N=109. Table 1, col(2): <[ILW2016] GHH-NNNNNN> N=47 among (Nos G09-47693 to G09-101355, G12-34009 to G12-87695, G15-21998 to G15-105504), <[ILW2016] SGP-NNNNNN> N=33 among (Nos 28124-499828), <[ILW2016] NGP-NNNNNN> N=32 among (Nos 63663-316031).
=E=	Catalogue in electronic form as <J/ApJ/832/78/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IM
IM	(IMACS)
*****	Avoid the usage of IM, prefer [MHI2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [IMB2008]
[IMB2008]
Write:	<<[IMB2008] A>> <<[IMB2008] radio core>>
N:	3+1
Object:	(smm) + (Rad) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	SMA 890µm and VLA 20cm observations of the field of 4C 60.07.
Ref:	=2008MNRAS.390.1117I
by	IVISON R.J. , MORRISON G.E., BIGGS A.D., SMAIL I., WILLNER S.P., GURWELL M.A., GREVE T.R., STEVENS J.A., ASHBY M.L.N.
	Mon. Not. R. Astron. Soc., 390, 1117-1126 (2008)
	Interferometric imaging of the high-redshift radio galaxy, 4C60.07: an SMA, Spitzer and VLA study reveals a binary AGN/starburst.
o	Text, Table 2: <[IMB2008] A> (Nos A-B, K). Table 2: <[IMB2008] radio core> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IML2013]
[IML2013]	(Ilbert+McCracken+Le Fevre+, 2013)
Write:	<<[IML2013] DDD.ddddd+DD.ddddd>>
N:	339384
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Sources without a match in the UltraVISTA DR1 catalog. Use of Subaru WFMOS and MOIRCS, and HST WFC3 data.
Ref:	=2013A&A...556A..55I
by	ILBERT O. , McCRACKEN H.J., LE FEVRE O., CAPAK P., DUNLOP J., KARIM A., RENZINI M.A., CAPUTI K., BOISSIER S., ARNOUTS S., AUSSEL H., COMPARAT J., GUO Q., HUDELOT P., KARTALTEPE J., KNEIB J.P., KROGAGER J.K., LE FLOC'H E., LILLY S., MELLIER Y., MILVANG-JENSEN B., MOUTARD T., ONODERA M., RICHARD J., SALVATO M., SANDERS D.B., SCOVILLE N., SILVERMAN J.D., TANIGUCHI Y., TASCA L., THOMAS R., TOFT S., TRESSE L., VERGANI D., WOLK M., ZIRM A.
	Astron. Astrophys., 556A, 55-55 (2013)
	Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTA.
o	uvista.dat: <[IML2013] DDD.ddddd+DD.ddddd> N=339384.
=E=	Catalogue in electronic form as J/A+A/556/A55
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IMM2000]
[IMM2000]	(Iwamuro+Motohara+Maihara+, 2000) (Not yet in Simbad)
Write:	<<[IMM2000] A>>
N:	5
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=5 objects in the HDF North
in source:	NAME HDFN
Ref:	=2000PASJ...52...73I
by	IWAMURO F. , MOTOHARA K., MAIHARA T., IWAI J., TANABE H., TAGUCHI T., HATA R., TERADA H., GOTO M., OYA S., IYE M., YOSHIDA M., KAROJI H., OGASAWARA R., SEKIGUCHI K.
	Publ. Astron. Soc. Jap., 52, 73-79 (2000)
	Near-infrared emission-line galaxies in the Hubble Deep Field North.
o	Table 2: <[IMM2000] A> (Nos A-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IMM2021]
[IMM2021]	(Ibata+Malhan+Martin+, 2021)
Write:	<<[IMM2021] C-NN>>
N:	26
Object:	Poss. Stellar Stream (SIMBAD class: Stream = Stellar Stream)
Stat:	is completely incorporated in Simbad
Note:	N=26 stellar stream candidates, using Gaia DR2 and EDR3 data. See also [MIM2018].
Ref:	=2021ApJ...914..123I
by	IBATA R. , MALHAN K., MARTIN N., AUBERT D., FAMAEY B., BIANCHINI P., MONARI G., SIEBERT A., THOMAS G.F., BELLAZZINI M., BONIFACIO P., CAFFAU E., RENAUD F.
	Astrophys. J., 914, 123-123 (2021)
	Charting the Galactic acceleration field. I. A search for stellar streams with Gaia DR2 and EDR3 with follow-up from ESPaDOnS and UVES.
o	<NAME Hrid Stream> N=1. <NAME Gunnthra Stream> N=1. <[MIM2018] Gaia-NN> (Nos 6-12) added. <[IMM2021] C-NN> (Nos 1-20).
Ref:	=2022MNRAS.516.5331M
by	MARTIN N.F. , IBATA R.A., STARKENBURG E., YUAN Z., MALHAN K., BELLAZZINI M., VISWANATHAN A., AGUADO D., ARENTSEN A., BONIFACIO P., CARLBERG R., GONZALEZ HERNANDEZ J.I., HILL V., JABLONKA P., KORDOPATIS G., LARDO C., McCONNACHIE A.W., NAVARRO J., SANCHEZ-JANSSEN R., SESTITO F., THOMAS G.F., VENN K.A., VITALI S., VOGGEL K.T.
	Mon. Not. R. Astron. Soc., 516, 5331-5354 (2022)
	The Pristine survey - XVI. The metallicity of 26 stellar streams around the Milky Way detected with the STREAMFINDER in Gaia EDR3.
o	<[IMM2021] C-NN> (Nos C-21 to C-26).
=E=	Catalogue in electronic form as <J/ApJ/914/123/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [IMO2013]
[IMO2013]	(Ichikawa+Matsushita+Okabe+, 2013)
Write:	<<[IMO2013] NN>>
N:	32
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Suzaku XIS and XMM-Newton MOS observations of N=32 sources in the field of the galaxy cluster ACO 1835.
in source:	ACO 1835
Ref:	=2013ApJ...766...90I
by	ICHIKAWA K. , MATSUSHITA K., OKABE N., SATO K., ZHANG Y.-Y., FINOGUENOV A., FUJITA Y., FUKAZAWA Y., KAWAHARADA M., NAKAZAWA K., OHASHI T., OTA N., TAKIZAWA M., TAMURA T., UMETSU K.
	Astrophys. J., 766, 90 (2013)
	Suzaku observations of the outskirts of A1835: deviation from hydrostatic equilibrium.
o	Table 11: <[IMO2013] NN> (Nos 1-32).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IMS
IMS	(Infrared Medium-deep Survey)
Write:	<<IMS JHHMMSS.ss+DDMMSS.s>> <<IMS JHHMMSS+DDMMSS>> <<IMS JHHMM+DDMM>> (not recognised by Simbad, but found in literature)
N:	1+6+49+13+43+25
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Note:	The Infrared Medium-deep Survey (IMS) is a moderately wide (120 square degrees) and moderately deep (J∼22.5-23mag) NIR imaging survey with UKIRT WFCAM. The IMS includes seven extragalactic fields (XMM-LSS, CFHTLS-W2, Lockman Hole, EGS, ELAIS-N1, ELAIS-N2, and SA22). Additional Gemini GNIRS and Magellan FIRE spectroscopy.
in source:	NAME XMM-LSS Field
in source:	NAME Lockman Hole
in source:	NAME Extended Groth Strip
in source:	ELAIS N1
in source:	ELAIS N2
in source:	SSA 22
Ref:	=2015ApJ...813L..35K
by	KIM Y. , IM M., JEON Y., KIM M., CHOI C., HONG J., HYUN M., JUN H.D., KAROUZOS M., KIM D., KIM D., KIM J.-W., KIM J.H., LEE S.-K., PAK S., PARK W.-K., TAAK Y.C., YOON Y.
	Astrophys. J., 813L, 35 (2015)
	Discovery of a faint quasar at z ~ 6 and implications for cosmic reionization.
o	Figs 2-3, Table 1: <IMS JHHMMSS.ss+DDMMSS.s> N=1.
Ref:	=2017ApJS..231...16J
by	JEON Y. , IM M., KIM D., KIM Y., JUN H.D., PAK S., TAAK Y.C., BAEK G., CHOI C., CHOI N., HONG J., HYUN M., JI T.-G., KAROUZOS M., KIM D., KIM J.-W., KIM J.H., KIM M., KIM S., LEE H.-I., LEE S.-K., PARK W.-K., PARK W., YOON Y.
	Astrophys. J., Suppl. Ser., 231, 16-16 (2017)
	The Infrared Medium-deep Survey. III. Survey of luminous quasars at 4.7 <= z <= 5.4.
o	Table 3: <IMS JHHMMSS.ss+DDMMSS.s> N=6.
Ref:	=2019ApJ...870...86K
by	KIM Y. , IM M., JEON Y., KIM M., PAK S., TAAK Y.C., CHOI C., HONG J., HYUN M., JI T.-G., JUN H.D., KAROUZOS M., KIM D., KIM D., KIM J.-W., KIM J.H., LEE H.-I., LEE S.-K., PARK W.-K., YOON Y., BYEON S., HWANG S., KIM J., KIM S., LIM G., PAEK I., PARK W., SHIN S.
	Astrophys. J., 870, 86-86 (2019)
	The Infrared Medium-deep Survey. VI. Discovery of faint quasars at z ~ 5 with a medium-band-based approach.
o	Tables 1-6: <IMS JHHMMSS+DDMMSS> N=49.
Ref:	=2020ApJ...893...45S
by	SHIN S. , IM M., KIM Y., HYUN M., PAK S., JEON Y., JI T.-G., AHN H., BYEON S., HAN J., HWANG S., KIM S., LIM G., PAEK I., PAEK G.S.H., TAAK Y.C., CHOI C., HONG J., JUN H.D., KIM D., KIM D., KIM M., KIM J.-W., KIM J.H., LEE H.-I., LEE S.-K., PARK W.-K., PARK W., YOON Y.
	Astrophys. J., 893, 45-45 (2020)
	The Infrared medium-deep survey. VII. Faint quasars at z ~ 5 in the ELAIS-N1 field.
o	Tables 1-3: <IMS JHHMMSS+DDMMSS> N=13.
Ref:	=2020ApJ...904..111K
by	KIM Y. , IM M., JEON Y., KIM M., PAK S., HYUN M., TAAK Y.C., SHIN S., LIM G., PAEK G.S.H., PAEK I., JIANG L., CHOI C., HONG J., JI T.-G., JUN H.D., KAROUZOS M., KIM D., KIM D., KIM J.-W., KIM J.H., LEE H.-I., LEE S.-K., PARK W.-K., YOON Y., BYEON S., HWANG S., KIM J., KIM S., PARK W.
	Astrophys. J., 904, 111-111 (2020)
	The Infrared Medium-deep Survey. VIII. Quasar luminosity function at z ~ 5.
o	Table 4: <IMS JHHMMSS+DDMMSS> N=43.
Ref:	=2022AJ....164..114K
by	KIM Y. , IM M., JEON Y., KIM M., JIANG L., SHIN S., CHOI C., HYUN M., JUN H.D., KIM D., KIM D., KIM J.-W., KIM J.H., LEE B., LEE S.-K., MOLINA J., PAK S., PARK W.-K., TAAK Y.C., YOON Y.
	Astron. J., 164, 114 (2022)
	The Infrared Medium-deep Survey. IX. Discovery of Two New z ~ 6 Quasars and Space Density Down to M_{1450} ~ -23.5 mag.
o	Table 2: <IMS JHHMMSS+DDMMSS> N=25.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [IMS2011]
[IMS2011]	(Iwasawa+Mazzarella+Surace+, 2011)
Write:	<<[IMS2011] CSCN>>
N:	3
Object:	Poss. Cluster of * (SIMBAD class: ClG_Candidate = Cluster of Galaxies Candidate)
Stat:	is completely incorporated in Simbad
Note:	N=3 candidate star clusters near the nuclear regions of Mrk 273. Use of archival HST ACS and NICMOS data from the Great Observatories All-sky LIRG Survey (GOALS). See also GOALS.
in source:	Mrk 273
Ref:	=2011A&A...528A.137I
by	IWASAWA K. , MAZZARELLA J.M., SURACE J.A., SANDERS D.B., ARMUS L., EVANS A.S., HOWELL J.H., KOMOSSA S., PETRIC A., TENG S.H., U V., VEILLEUX S.
	Astron. Astrophys., 528A, 137-137 (2011)
	The location of an active nucleus and a shadow of a tidal tail in the ULIRG Mrk 273.
o	Paragr. 3.1: <[IMS2011] CSCN> (Nos CSC1-CSC3) = <GOALS JHHMMSS.ss+DDMMSS.s> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IMS2012]
[IMS2012]	(Immer+Menten+Schuller+, 2012)
Write:	<<[IMS2012] A>> (SIMBAD class: Radio = Radio Source)
Note:	VLA 8.4GHz observations of the Galactic center dust ridge.
Ref:	=2012A&A...548A.120I
by	IMMER K. , MENTEN K.M., SCHULLER F., LIS D.C.
	Astron. Astrophys., 548A, 120-120 (2012)
	A multi-wavelength view of the Galactic Center dust ridge reveals little star formation.
o	Tables 3,4 : <[IMS2012] A> (Nos A-E) N=5
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IMSCl
IMSCl	(Infrared Medium-deep Survey Cluster)
Write:	<<IMSCl JHHMM+DDMM>>
N:	3
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Magellan IMACS spectroscopy of N=3 galaxy clusters at z∼0.91 in the SSA22 field, as part of the Infrared Medium-deep Survey (IMS). See also [KIL2016].
in source:	SSA 22
Ref:	=2016ApJ...821L..10K
by	KIM J.-W. , IM M., LEE S.-K., EDGE A.C., HYUN M., KIM D., CHOI C., HONG J., JEON Y., JUN H.D., KAROUZOS M., KIM D., KIM J.H., KIM Y., PARK W.-K., TAAK Y.C., YOON Y.
	Astrophys. J., 821L, 10-10 (2016)
	Discovery of a supercluster at z ~ 0.91 and testing the ΛCDM cosmological model.
o	<[KIL2016] Cl J2213> N=1. Fig. 2, Table 1: <IMSCl JHHMM+DDMM> N=3.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [IMT2005]
[IMT2005]	(Inui+Matsumoto+Tsuru+, 2005)
Write:	<<[IMT2005] NN>>
N:	67
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of NGC 2146.
in source:	NGC 2146
Ref:	=2005PASJ...57..135I
by	INUI T. , MATSUMOTO H., TSURU T.G., KOYAMA K., MATSUSHITA S., PECK A.B., TARCHI A.
	Publ. Astron. Soc. Jap., 57, 135-145 (2005)
	Chandra observation of the starburst galaxy NGC 2146.
o	Table 8: <[IMT2005] NN> (Nos 1-67).
=E=	Catalogue in electronic form as J/PASJ/57/135
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IMT2006]
[IMT2006]	(Isobe Makishima+Tashiro+, 2006)
Write:	<<[IMT2006] NN>>
N:	59
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton observations of Fornax A radio galaxy.
in source:	NGC 1316 = For A
Ref:	=2006ApJ...645..256I
by	ISOBE N. , MAKISHIMA K., TASHIRO M., ITOH K., IYOMOTO N., TAKAHASHI I., KANEDA H.
	Astrophys. J., 645, 256-263 (2006)
	The XMM-Newton examination of energetics in the east lobe of the nearby radio galaxy Fornax A (NGC 1316).
o	Table 2: <[IMT2006] NN> (Nos 1-59).
=E=	Catalogue in electronic form as J/ApJ/645/256
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IN88]
[IN88]	(Impey+Neugebauer, 1988)
Write:	<<[IN88] HHMM+DDd>>
N:	165
Object:	Blazar (SIMBAD class: Blazar)
Stat:	is completely incorporated in Simbad
Note:	IRAS observations of 165 Blazars. The letter 'a' added at the end of the format denotes several observations of the same object 'HHMM+DDd',
Ref:	=1988AJ.....95..307I
by	IMPEY C.D. , NEUGEBAUER G.
	Astron. J., 95, 307-351 (1988)
	Energy distributions of blazars.
o	Table I: <[IN88] HHMM+DDd> N=165.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: INCA
INCA	((Hipparcos) Input Catalogue)
*****	Avoid the usage of INCA, prefer HIC
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [INI2020]
[INI2020]	(Izumi+Nguyen+Imanishi+, 2020)
Write:	<<[INI2020] A>>
N:	4
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 7 (860µm) continuum observations of N=4 submillimeter sources toward the AGN of NGC 7649.
in source:	NGC 7469
Ref:	=2020ApJ...898...75I
by	IZUMI T. , NGUYEN D.D., IMANISHI M., KAWAMURO T., BABA S., NAKANO S., KOHNO K., MATSUSHITA S., MEIER D.S., TURNER J.L., MICHIYAMA T., HARADA N., MARTIN S., NAKANISHI K., TAKANO S., WIKLIND T., NAKAI N., HSIEH P.-Y.
	Astrophys. J., 898, 75-75 (2020)
	ALMA observations of multiple CO and C lines toward the active galactic nucleus of NGC 7469: an X-ray-dominated region caught in the act.
o	Fig. 2, Table 6: <[INI2020] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [INM2011]
[INM2011]	(Ikeda+Nagao+Matsuoka+, 2011) (Not yet in Simbad)
Write:	<<[INM2011] N>>
N:	8
Object:	QSO (SIMBAD class: QSO = Quasar)
Note:	Subaru FOCAS observations of N=8 quasars in the COSMOS field.
in source:	NAME COSMOS Field
Ref:	=2011ApJ...728L..25I
by	IKEDA H. , NAGAO T., MATSUOKA K., TANIGUCHI Y., SHIOYA Y., TRUMP J.R., CAPAK P., COMASTRI A., ENOKI M., IDEUE Y., KAKAZU Y., KOEKEMOER A.M., MOROKUMA T., MURAYAMA T., SAITO T., SALVATO M., SCHINNERER E., SCOVILLE N.Z., SILVERMAN J.D.
	Astrophys. J., 728L, 25 (2011)
	Probing the faint end of the quasar luminosity function at z~ 4 in the COSMOS field.
o	Table 1: <[INM2011] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: INN
INN	(Innes)= (Innes)
Write:	<<*SV INN** NNN>>
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Rem:	V* Nomenclature.
Details on Acronym: Innes
Innes	(Innes)
*****	Avoid the usage of Innes, prefer INN
Details on Acronym: [INS2001]
[INS2001]	(Ishii+Nagata+Sato+, 2001)
Write:	<<[INS2001] JHHMMSS.s+DDMMSS>>
N:	11
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=4 brightest sources part of CPM binary YSO or of CPM cluster. N=7 nearby stars from CPM YSOs.
Ref:	=2001AJ....121.3191I
by	ISHII M. , NAGATA T., SATO S., YAO Y., JIANG Z., NAKAYA H.
	Astron. J., 121, 3191-3206 (2001)
	K-band spectroscopy of luminous young stellar objects.
o	Par. 4.1.1., CPD -57 2824 misprint for CPD -57 2874.
o	Appendix: <[INS2001] JHHMMSS.s+DDMMSS> N=4+7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [INS2019]
[INS2019]	(Ishii+Nakamura+Shimajiri+, 2019)
Write:	<<[INS2019] NN>>
N:	78
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	Nobeyama 45m telescope 13CO(1-0) observations of N=78 clouds towards Orion A Giant Molecular Cloud.
in source:	NAME Ori A
Ref:	=2019PASJ...71S...9I
by	ISHII S. , NAKAMURA F., SHIMAJIRI Y., KAWABE R., TSUKAGOSHI T., DOBASHI K., SHIMOIKURA T.
	PASJ, 71S, 9 (2019)
	Nobeyama 45 m mapping observations towardOrion A. II. Classification of cloud structures and variation of the ^{13}CO/C{18}O abundance ratio dueto far-UV radiation.
o	Fig. 3, Tables 3-4: <[INS2019] NN> (Nos 1-78).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [INS97]
[INS97]	(Itoh+Nakada+Soyano+, 1997)= (OT)
Write:	<<[INS97] JHHMMSS.s+DDMMSS.s>> <<[INS97] JHHMMSS.ss+DDMMSS.s>>
N:	2
Object:	(Rad) + OT (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	New objects in the error box of GRB 971214: N=1 faint source: J115625.2+651157.9 N=1 Optical Transient: J115626.40+651200.5 = OT 19971214
Ref:	=1997IAUC.6788Q...1I
by	ITOH N. , NAKADA Y., SOYANO T., HALPERN J., THORSTENSEN J., HELFAND D., COSTA E., (The BeppoSAX Team)
	IAU Circ., 6788, 1-None (1997)
	GRB 971214.
o	<[INS97] J115625.2+651157.9>, <[INS97] J115626.40+651200.5>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: INT
INT	(Aden+Feltzing+Koch+, 2009) (Not yet in Simbad)
*****	Avoid the usage of INT, prefer [AFK2009]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [INT2003]
[INT2003]	(Imanishi+Nakajima+Tsujimoto+, 2003)
Write:	<<[INT2003] A-NN>> <<[INT2003] {A}-{S\|H}N>> <<[INT2003] BF-NN>> <<[INT2003] {BF}-{S\|H}N>>
N:	84+5+5+98+*+4
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra X-ray sources in rho Oph cloud study. Search for systematic flares from YSO. The letters 'A' and 'BF' in the first part of the format stand for observations centered on [LWS80] rho Oph A and [LWS80] rho Oph B to F cores, the letters 'S' and 'H' in the second part of the format stand for sources observed only in Soft bands or in Hard bands.
in source:	NAME rho Oph Cloud
Ref:	=2003PASJ...55..653I
by	IMANISHI K. , NAKAJIMA H., TSUJIMOTO M., KOYAMA K., TSUBOI Y.
	Publ. Astron. Soc. Jap., 55, 653-681 (2003)
	A systematic study of X-ray flares from low-mass young stellar objects in the ρ Ophiuchi star-forming region with Chandra.
o	Table 2: <[INT2003] A-NN> (Nos A-1 to A-84), <[INT2003] A-AN> (Nos A-S1 to A-S5, A-H1 to A-H5), <[INT2003] AA-NN> (Nos BF-1 to BF-98), <[INT2003] AA-AN> (Nos BF-S1 to BF-S8, BF-H1 to BF-H4).
=E=	Catalogue in electronic form as J/PASJ/55/653
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: INTEGRAL1
INTEGRAL1	(INTEGRAL, 1st results)= ([BBB2004b])
Write:	<<INTEGRAL1 NNN>>
N:	123
Object:	(Soft Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Stat:	is completely incorporated in Simbad
Note:	First high-energy survey obtained with IBIS (Imager on Board INTEGRAL) in gamma-ray, for the Galactic Plane.
Ref:	=2004ApJ...607L..33B
by	BIRD A.J. , BARLOW E.J., BASSANI L., BAZZANO A., BODAGHEE A., CAPITANIO F., COCCHI M., DEL SANTO M., DEAN A.J., HILL A.B., LEBRUN F., MALAGUTI G., MALIZIA A., MUCH R., SHAW S.E., STEPHEN J.B., TERRIER R., UBERTINI P., WALTER R.
	Astrophys. J., 607, 33-37 (2004)
	The first IBIS/ISGRI soft γ-ray galactic plane survey catalog.
o	Table 1: <INTEGRAL1 NNN> (Nos 1-123).
=E=	Catalogue in electronic form as J/ApJ/607/L33
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: INTREF
INTREF	(INTEGRAL, Reference catalog)
Write:	<<INTREF NNNN>>
N:	1122
Object:	(X) + (Gamma) (SIMBAD class: gamma = Gamma-ray Source)
Note:	INTEGRAL reference catalog which classifies sources before the launch of INTEGRAL mission. See also IGR for final catalog.
Ref:	=2003A&A...411L..59E
by	EBISAWA K. , BOURBAN G., BODAGHEE A., MOWLAVI N., COURVOISIER T.J.-L.
	Astron. Astrophys., 411, 59-62 (2003)
	High-energy sources before INTEGRAL. INTEGRAL reference catalog.
o	Catalogue: <INTREF NNNN> (Nos 1-1122).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: INVS
INVS	(IGPS Narrow Vertical Structure survey)
Write:	<<INVS GLLL.l+BB.b+VVV>>
N:	10
Object:	HI vertical (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	INVS=International galactic plane survey Narrow Vertical structure Survey. Search for narrow vertical structures in HI cubes of the Canadian Galactic Plane Survey (CGPS).
Notes:	International Plane Survey (IGPS, http://www.ras.ucalgary.ca/IGPS/) we use HI cubes from the Canadian Galactic Plane Survey (CGPS) for our search. In "INVS", "Narrow" stands for a width:length ratio of 1:3, and "vertical" represents that most objects make > 45 degrees to the Galactic plane. The main idea is to convey that the object stands out of the plane, motivated by our study of the disk-halo connection. The position quoted belongs to the end of the object that is closest to the Galactic plane. The velocity quoted is the centroid of velocities. If one object has more then one Gaussians, one would quote the center of the dominant component. The total number of these objects may increase, depending upon similar searches in the future.
Ref:	=2005AJ....130..674A
by	ASGEKAR A. , ENGLISH J., SAFI-HARB S., KOTHES R.
	Astron. J., 130, 674-697 (2005)
	A search for narrow vertical structures in the Canadian Galactic plane survey.
o	Table 1: <INVS GLLL.l+B.b+VVV> N=10. Table 1: <[AES2005] GLLL+B.b+VVV>, <[AES2005] GLLL.l+B.b+VVV>, N=7.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [IOB2006]
[IOB2006]	(Inada+Oguri+Becker+, 2006)
Write:	<<[IOB2006] SDSS JHHMM+DDMM>> <<[IOB2006] SDSS JHHMM+DDMM A>> <<[IOB2006] SDSS JHHMM+DDMM AN>>
N:	2+2+1+4+3+1
Object:	Grav. lens system + Grav. lensed image of a QSO + Grav. lens + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Discovery of 2 lensed QSOs in SDSS, with follow up Keck II spectroscopic observations: SDSS J080623.70+200631.9: 2 images A and B and a lens galaxy G, and 4 galaxies surounding the QSO G1 to G4. SDSS J135306.35+113804.8: 3 images A to C and a lens galaxy G.
Ref:	=2006AJ....131.1934I
by	INADA N. , OGURI M., BECKER R.H., WHITE R.L., GREGG M.D., SCHECHTER P.L., KAWANO Y., KOCHANEK C.S., RICHARDS G.T., SCHNEIDER D.P., BARENTINE J.C., BREWINGTON H.J., BRINKMANN J., HARVANEK M., KLEINMAN S.J., KRZESINSKI J., LONG D., NEILSEN E.H.Jr, NITTA A., SNEDDEN S.A., YORK D.G.
	Astron. J., 131, 1934-1941 (2006)
	SDSS J0806+2006 and SDSS J1353+1138: two new gravitationally lensed quasars from the Sloan Digital Sky Survey.
o	Text: <[IOB2006] SDSS JHHMM.DDMM> N=2. Fig.3, Table 1: <[IOB2006] SDSS J0806+2006 A> (Nos A-B, G). Table 4: <[IOB2006] SDSS J0806+2006 AN> (Nos G1-G4). Figs 5,6, Table 5: <[IOB2006] SDSS J1353+1138 A> (Nos A-C, G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IOB2007]
[IOB2007]	(Inada+Oguri+Becker+, 2007)
Write:	<<[IOB2007] SDSS JHHMM+DDMM>> <<[IOB2007] SDSS JHHMM+DDMM A>> <<[IOB2007] QSO JHHMM+DDMM abs N.NN>>
N:	2+3+3+2+3
Object:	Grav. lens system + Grav. lensed image of a QSO + Grav. lens + ALS (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Discovery of 2 lensed QSOs in SDSS, with follow up UH88 photometric and Keck II spectroscopic observations: SDSS J074653.03+440351.3 and SDSS J140624.82+612640.9: each with 2 images A and B and a lens galaxy G.
Ref:	=2007AJ....133..206I
by	INADA N. , OGURI M., BECKER R.H., WHITE R.L., KAYO I., KOCHANEK C.S., HALL P.B., SCHNEIDER D.P., YORK D.G., RICHARDS G.T.
	Astron. J., 133, 206-213 (2007)
	Two new gravitationally lensed double quasars from the Sloan Digital Sky Survey.
o	Text: <[IOB2007] SDSS JHHMM+DDMM> N=2. Table 2: <[IOB2007] SDSS J0746+4403 A> (Nos A-B, G). Fig.3: <[IOB2007] QSO J0746+4403 abs N.NN> N=2. Table 4: <[IOB2007] SDSS J1406+6126 A> (Nos A-B, G). Fig.5: <[IOB2007] QSO J1406+6126 abs N.NN> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IOK
IOK	(Iye+Ota+Kashikawa+)
Write:	<<IOK N>> <<IOK Obj-N>> (not recognised by Simbad, but found in literature)
N:	5
Object:	LAE G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Subaru Suprime-Cam and FOCAS observations. Search for galaxies with z about 7.
Ref:	=2006Natur.443..186I
by	IYE M. , OTA K., KASHIKAWA N., FURUSAWA H., HASHIMOTO T., HATTORI T., MATSUDA Y., MOROKUMA T., OUCHI M., SHIMASAKU K.
	Nature, 443, 186-188 (2006)
	A galaxy at a redshift z = 6.96.
o	Fig.1, Table 1: <IOK N> (Nos 1-3).
Ref:	=2008ApJ...677...12O
by	OTA K. , IYE M., KASHIKAWA N., SHIMASAKU K., KOBAYASHI M., TOTANI T., NAGASHIMA M., MOROKUMA T., FURUSAWA H., HATTORI T., MATSUDA Y., HASHIMOTO T., OUCHI M.
	Astrophys. J., 677, 12-26 (2008)
	Reionization and galaxy evolution probed by z = 7 Lyα emitters.
o	Table 1: <IOK N> (Nos 4-5) added.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [IOK2007]
[IOK2007]	(Ishihara+Onaka+Kaneda+, 2007)
Write:	<<[IOK2007] A>>
N:	11
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	AKARI IR observations of IC 4954 and IC 4955.
in source:	IC 4954
in source:	IC 4955
Ref:	=2007PASJ...59S.443I
by	ISHIHARA D. , ONAKA T., KANEDA H., SUZUKI T., KATAZA H., SAKON I., OKADA Y., DOI Y., FUJISHIRO N., FUJIWARA H., ITA Y., KII T., KIM W., MAKIUTI S., MATSUMOTO T., MATSUHARA H., MURAKAMI H., NAKAGAWA T., OHYAMA Y., OYABU S., SERJEANT S., SHIBAI H., TAKAGI T., TANABE T., UEMIZU K., UENO M., USUI F., WADA T., WATARAI H., YAMAMURA I.
	PASJ, 59S, 443-454 (2007)
	AKARI infrared imaging of reflection nebulae IC4954 and IC4955.
o	Stars in fig.4 are not in Simbad
o	Table 3: <[IOK2007] A> (Nos A-L).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IOM2006]
[IOM2006]	(Inada+Oguri+Morokuma+, 2006)
Write:	<<[IOM2006] SDSS J1029+2623>> <<[IOM2006] SDSS J1029+2623 A>> <<[IOM2006] Lensing Cluster>> <<[IOM2006] GNa>>
N:	3+1+2+2+2
Object:	Grav. lens system + Grav. lensed image of a QSO + Grav. lens + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Subaru FOCAS, Keck I LRIS, and UH88 observations of the lensed QSO SDSS J102913.94+262317.9: N=3 lensed images A to C, the lens is a cluster of galaxies divided into N=2 bright galaxies G1 and G2, both resolved in turn into 2 components.
Ref:	=2006ApJ...653L..97I
by	INADA N. , OGURI M., MOROKUMA T., DOI M., YASUDA N., BECKER R.H., RICHARDS G.T., KOCHANEK C.S., KAYO I., KONISHI K., UTSUNOMIYA H., SHIN M.-S., STRAUSS M.A., SHELDON E.S., YORK D.G., HENNAWI J.F., SCHNEIDER D.P., DAI X., FUKUGITA M.
	Astrophys. J., 653L, 97-100 (2006)
	SDSS J1029+2623: a gravitationally lensed quasar with an image separation of 22.5".
o	Fig.1, Table 1: <[IOM2006] J1029+2623 A> (Nos A-B), <[IOM2006] Lensing Cluster> N=1, <[IOM2006] GN> (Nos G1-G2).
Ref:	=2008ApJ...676L...1O
by	OGURI M. , OFEK E.O., INADA N., MOROKUMA T., FALCO E.E., KOCHANEK C.S., KAYO I., BROADHURST T., RICHARDS G.T.
	Astrophys. J., 676L, 1-4 (2008)
	The third image of the large-separation lensed quasar SDSS J1029+2623.
o	Table 1: <[IOM2006] J1029+2623 A> (No. C) added, <[IOM2006] GNa> (Nos G1a, G1b).
Ref:	=2011ApJ...728L..18K
by	KRATZER R.M. , RICHARDS G.T., GOLDBERG D.M., OGURI M., KOCHANEK C.S., HODGE J.A., BECKER R.H., INADA N.
	Astrophys. J., 728L, 18 (2011)
	Analyzing the flux anomalies of the large-separation lensed quasar SDSS J1029+2623.
o	Fig. 1, Table 1: <[IOM2006] G2a> (Nos G2a-G2b) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IOMC
IOMC	(INTEGRAL OPTICAL MONITORING CAMERA) (Not yet in Simbad)
Write:	<<IOMC FFFFNNNNNN>>
N:	about 500000
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	In preparation. The Optical Monitoring Camera (OMC) onboard INTEGRAL (launched on October 17, 2002) has been designed to obtain V-Johnson photometry. Due to technical limitations on the data processing electronics and the available telemetry, it is necessary to know, a priori, the objects to be monitored within the field of view (FOV) of the OMC. The OMC Input Catalogue, and subsequent updates, provides this information: astrometric and photometric reference stars for calibration and scientific targets for accurate photometric variability studies.
Auth.:	DOMINGO A.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [IOP2003]
[IOP2003]	(Inada+Oguri+Pindor+, 2003)
Write:	<<[IOP2003] SDSS J1004+4112>> <<[IOP2003] SDSS J1004+4112 A>> <<[IOP2003] G>> <<[IOP2003] Cluster>>
N:	1+5+1+1
Object:	Grav. lens system + Grav. lensed image + G + Cluster of G + Grav. lens (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Study of the gravitationally lensed QSO J1004+4112. N=5 lensed images of the QSO, (Nos A-E), N=1 galaxy between the images, the brightest galaxy of the lensing Cluster. See also [OIK2004]
Ref:	=2003Natur.426..810I
by	INADA N. , OGURI M., PINDOR B., HENNAWI J.F., CHIU K., ZHENG W., ICHIKAWA S.-I., GREGG M.D., BECKER R.H., SUTO Y., STRAUSS M.A., TURNER E.L., KEETON C.R., ANNIS J., CASTANDER F.J., EISENSTEIN D.J., FRIEMAN J.A., FUKUGITA M., GUNN J.E., JOHNSTON D.E., KENT S.M., NICHOL R.C., RICHARDS G.T., RIX H.-W., SHELDON E.S., BAHCALL N.A., BRINKMANN J., IVEZIC Z., LAMB D.Q., McKAY T., SCHNEIDER D.P., YORK D.G.
	Nature, 426, 810-812 (2003)
	A gravitationally lensed quasar with quadruple images separated by 14.62 arcseconds.
o	<[IOP2003] J1004+4112 A> (Nos A-D), <[IOP2003] G> N=1, <[IOP2003] Cluster> N=1, <[IOP2003] SDSS J1004+4112> N=1.
Ref:	=2005PASJ...57L...7I
by	INADA N. , OGURI M., KEETON C.R., EISENSTEIN D.J., CASTANDER F.J., CHIU K., HALL P.B., HENNAWI J.F., JOHNSTON D.E., PINDOR B., RICHARDS G.T., RIX H.-W.R., SCHNEIDER D.P., ZHENG W.
	Publ. Astron. Soc. Jap., 57, 7-10 (2005)
	Discovery of a fifth image of the large separation gravitationally lensed quasar SDSS J1004+4112.
o	Table 1: <[IOP2003] J1004+4112 A> (No. E) added. Fig.2: <[OIK2004] GN> (No. G4) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IOR2014]
[IOR2014]	(Inada+Oguri+Rusu+, 2014)
Write:	<<[IOR2014] SDSS JHHMM+DDMM>> <<[IOR2014] SDSS JHHMM+DDMM AN>>
N:	4+13
Object:	Grav. lens system + Grav. lens + Grav. lensed image of a QSO
Stat:	is completely incorporated in Simbad
Note:	UH88 2.2m telescope, ARC 3.5m telescope, TNG 3.58m telescope, Subaru 8.2m telescope, and Gemini North 8.1m telescope observations of N=4 gravitational lens systems, selected from SDSS data.
Ref:	=2014AJ....147..153I
by	INADA N. , OGURI M., RUSU C.E., KAYO I., MOROKUMA T.
	Astron. J., 147, 153 (2014)
	Discovery of four doubly imaged quasar lenses from the Sloan Digital Sky Survey.
o	(Erratum) erratum vol. 149, art. 35 (2015)
o	Figs 1-2, Table 1: <[IOR2014] SDSS JHHMM+DDMM> N=4. Table 5: <[IOR2014] SDSS JHHMM+DDMM AN> N=3+3+4+3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IOS2009]
[IOS2009]	(Inada+Oguri+Shin+, 2009)
Write:	<<[IOS2009] SDSS JHHMM+DDMM>> <<[IOS2009] SDSS JHHMM+DDMM A>>
N:	5+16
Object:	? + QSO + Grav. lensed image of a QSO + Grav. lens (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Discovery of N=5 lensed quasars from the SDSS. Additional observations with UH88, ARC 3.5m and TNG 3.6m telescopes.
Ref:	=2009AJ....137.4118I
by	INADA N. , OGURI M., SHIN M.-S., KAYO I., STRAUSS M.A., MOROKUMA T., SCHNEIDER D.P., BECKER R.H., BAHCALL N.A., YORK D.G.
	Astron. J., 137, 4118-4126 (2009)
	Five new high-redshift quasar lenses from the Sloan Digital Sky Survey.
o	Text: <[IOS2009] SDSS JHHMM+DDMM> N=5. Table 5: <[IOS2009] SDSS JHHMM+DDMM A> N=16.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IOT2002]
[IOT2002]	(Ikeda+Oka+Tatematsu+, 2002) (Not yet in Simbad)
Write:	<<[IOT2002] A>>
N:	24
Object:	Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud)
Note:	CI peaks in ORI GMC.
in source:	NAME Ori GMC
Ref:	=2002ApJS..139..467I
by	IKEDA M. , OKA T., TATEMATSU K., SEKIMOTO Y., YAMAMOTO S.
	Astrophys. J., Suppl. Ser., 139, 467-485 (2002)
	The distribution of atomic carbon in the Orion giant molecular cloud 1.
o	Figs 7, 8 and Tables 3, 4: regions are not in SIMBAD.
o	Figs 5, 6: <[IOT2002] A> (Nos A-X).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IOT2007]
[IOT2007]	(Iwata+Ohta+Tamura+, 2007)
Write:	<<[IOT2007] NNNNNN>>
N:	11+105
Object:	EmG (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Subaru Suprime-Cam and FOCAS observations. Search for Lyman Break Galaxies.
Ref:	=2007MNRAS.376.1557I
by	IWATA I. , OHTA K., TAMURA N., AKIYAMA M., AOKI K., ANDO M., KIUCHI G., SAWICKI M.
	Mon. Not. R. Astron. Soc., 376, 1557-1576 (2007)
	Differential evolution of the UV luminosity function of Lyman break galaxies from z ~ 5 to 3.
o	In chap 3.4 : CDFa-GD12 is a misprint for CDFb-GD12.
o	Tables 3,4: <[IOT2007] NNNNNN> N=11.
Ref:	=2009ApJ...693..507Y
by	YABE K. , OHTA K., IWATA I., SAWICKI M., TAMURA N., AKIYAMA M., AOKI K.
	Astrophys. J., 693, 507-533 (2009)
	The stellar populations of Lyman break galaxies at z ~ 5.
o	Tables 1, 2: <[IOT2007] NNNNNN> N=105.
=E=	Catalogue in electronic form as <J/ApJ/693/507/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IOT2010]
[IOT2010]	(Ita+Onaka+Tanabe+, 2010)
Write:	<<[IOT2010] DDD.dddddd+DD.dddddd>>
N:	26365
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	AKARI IRC near- to mid-infrared imaging and spectroscopic observations of the Small Magellanic Cloud.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2010PASJ...62..273I
by	ITA Y. , ONAKA T., TANABE T., MATSUNAGA N., MATSUURA M., YAMAMURA I., NAKADA Y., IZUMIURA H., UETA T., MITO H., FUKUSHI H., KATO D.
	PASJ, 62, 273-286 (2010)
	AKARI near- to mid-infrared imaging and spectroscopic observations of the Small Magellanic Cloud. I Bright point source list.
o	Table 2: <[IOT2010] DDD.dddddd+DD.dddddd> N=26365.
=E=	Catalogue in electronic form as J/PASJ/62/273
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IOZ2018]
[IOZ2018]	(Itoh +Ouchi+Zhang+, 2018)
Write:	<<[IOZ2018] HSC-z7LAENN>>
N:	34
Object:	Poss. LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	Subaru HSC observations of N=34 LAE candidates at z=7 in the SXDS and COSMOS fields, as part of the Cosmic HydrOgen Reionization Unveiled with Subaru (CHORUS) project.
in source:	NAME COSMOS Field
in source:	NAME SXDSF
Ref:	=2018ApJ...867...46I
by	ITOH R. , OUCHI M., ZHANG H., INOUE A.K., MAWATARI K., SHIBUYA T., HARIKANE Y., ONO Y., KUSAKABE H., SHIMASAKU K., FUJIMOTO S., IWATA I., KAJISAWA M., KASHIKAWA N., KAWANOMOTO S., KOMIYAMA Y., LEE C.-H., NAGAO T., TANIGUCHI Y.
	Astrophys. J., 867, 46-46 (2018)
	CHORUS. II. Subaru/HSC determination of the Lyα luminosity function at z = 7.0: constraints on Cosmic reionization model parameter.
o	Table 2: <[IOZ2018] HSC-z7LAENN> (Nos 1-34).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IPA98]
[IPA98]	(Immler+Pietsch+Aschenbach, 1998)
Write:	<<[IPA98] HNN>> <<[IPA98] ENN>>
N:	33+15
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI and Einstein observations. Table 2: (Nos H1-H33), ROSAT HRI X-ray sources. Table 3: (Nos E1-E15), Einstein X-ray sources. Cross-identifications betwen the two formats.
in source:	NGC 4321
Ref:	=1998A&A...331..601I
by	IMMLER S. , PIETSCH W., ASCHENBACH B.
	Astron. Astrophys., 331, 601-611 (1998)
	X-ray emission from NGC 4321 (M 100): detection of supernova 1979C.
o	CB 336 = [CB90] 336
o	Table 2: <[IPA98] HNN> (Nos H1-H33). Table 3: <[IPA98] ENN> (Nos E1-E15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IPC
IPC	(Imaging Proportional Counter)
*****	Avoid the usage of IPC, prefer 2E
Origin	of the Acronym: L = Found in the literature
Details on Acronym: IPC
IPC	(Imaging Proportional Counter)
*****	Avoid the usage of IPC, prefer [TSA98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [IPE92]
[IPE92]	(Ivanov+Popravko+Efremov+, 1992)
Write:	<<[IPE92] OBNNN>>
N:	147
Object:	Assoc. (SIMBAD class: Association = Association of Stars)
Stat:	is completely incorporated in Simbad
in source:	NGC 628 = M 74
Ref:	=1992A&AS...96..645I
by	IVANOV G.R. , POPRAVKO G., EFREMOV Y.N., TICHONOV N.A., KARACHENTSEV I.D.
	Astron. Astrophys., Suppl. Ser., 96, 645-652 (1992)
	Stellar associations and aggregates in NGC 628.
o	<[IPE92] OBNNN> N=147
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IPG2004]
[IPG2004]	(Izotov+Papaderos+Guseva+, 2004)
Write:	<<[IPG2004] gN>>
N:	8
Object:	G (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT/FORS spectroscopic observations of the field of Tol 1214-277 and Tol 65. N=4 galaxies in each field.
Ref:	=2004A&A...421..539I
by	IZOTOV Y.I. , PAPADEROS P., GUSEVA N.G., FRICKE K.J., THUAN T.X.
	Astron. Astrophys., 421, 539-554 (2004)
	Deep VLT spectroscopy of the blue compact dwarf galaxies Tol 1214-277 and Tol 65.
o	Table 7: <[IPG2004] gN> (Nos g1-g8).
=E=	Catalogue in electronic form as J/A+A/421/539
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IPG2006]
[IPG2006]	(Izotov+Papaderos+Guseva+, 2006) (Not yet in Simbad)
Write:	<<[IPG2006] JHHMM+DDMM>> <<[IPG2006] J2104-0035W>> <<[IPG2006] J2104-0035 star>> <<[IPG2006] J0113+0052 BG>>
N:	3+2
Object:	G (SIMBAD class: Galaxy)
Note:	ESO telescope image of 2 SDSS emission-line galaxies.
Ref:	=2006A&A...454..137I
by	IZOTOV Y.I. , PAPADEROS P., GUSEVA N.G., FRICKE K.J., THUAN T.X.
	Astron. Astrophys., 454, 137-141 (2006)
	Two extremely metal-poor emission-line galaxies in the Sloan Digital Sky Survey.
o	J2104-0035 = J2104-0035C = SDSS J210455.31-003522.3, J0113+0052 = SDSS J011340.45+005239.1.
o	Figs 1: <[IPG2006] JHHMM+DDMM> N=2, <[IPG2006] J2104-0035W> (Nos C, N), <[IPG2006] J2104-0035 star> N=1, <[IPG2006] J0113+0052 BG> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IPHAS
IPHAS	(INT-WFC Photometric H-alpha Survey)
Write:	<<IPHAS JHHMMSS.ss+DDMMSS.s>>
N:	218991524
Object:	* (SIMBAD class: Star)
Note:	Point source catalog of a survey of the Northern Galactic Plane over a Galactic latitude range -5<b<+5, using the Wide Field Camera mounted on the Isaac Newton Telescope. Three filters are used: H-alpha, Sloan r, and Sloan i. Website: http://www.iphas.org/ 2005MNRAS.362..753D: primary reference for defining the survey, N∼80 million sources. 2008MNRAS.388...89G: Initial Data Release, N∼200 million sources. 2014MNRAS.444.3230B: Second Data Release, N=218 991 524 sources. See also IPHASX, UVEX.
Ref:	=2005MNRAS.362..753D
by	DREW J.E. , GREIMEL R., IRWIN M.J., AUNGWEROJWIT A., BARLOW M.J., CORRADI R.L.M., DRAKE J.J., GANSICKE B.T., GROOT P., HALES A., HOPEWELL E.C., IRWIN J., KNIGGE C., LEISY P., LENNON D.J., MAMPASO A., MASHEDER M.R.W., MATSUURA M., MORALES-RUEDA L., MORRIS R.A.H., PARKER Q.A., PHILLIPPS S., RODRIGUEZ-GIL P., ROELOFS G., SKILLEN I., SOKOLOSKI J.L., STEEGHS D., UNRUH Y.C., VIIRONEN K., VINK J.S., WALTON N.A., WITHAM A., WRIGHT N., ZIJLSTRA A.A., ZURITA A.
	Mon. Not. R. Astron. Soc., 362, 753-776 (2005)
	The INT Photometric Hα Survey of the Northern Galactic Plane (IPHAS).
o	Shajn 147 SNR = SIM 147
o	Text, Tables 5,6: <IPHAS JHHMMSS.ss+DDMMSS.s> N=15.
Ref:	=2008MNRAS.388...89G
by	GONZALEZ-SOLARES E.A. , WALTON N.A., GREIMEL R., DREW J.E., IRWIN M.J., SALE S.E., ANDREWS K., AUNGWEROJWIT A., BARLOW M.J., VAN DEN BESSELAAR E., CORRADI R.L.M., GANSICKE B.T., GROOT P.J., HALES A.S., HOPEWELL E.C., HU H., IRWIN J., KNIGGE C., LAGADEC E., LEISY P., LEWIS J.R., MAMPASO A., MATSUURA M., MOONT B., MORALES-RUEDA L., MORRIS R.A.H., NAYLOR T., PARKER Q.A., PREMA P., PYRZAS S., RIXON G.T., RODRIGUEZ-GIL P., ROELOFS G., SABIN L., SKILLEN I., SUSO J., TATA R., VIIRONEN K., VINK J.S., WITHAM A., WRIGHT N.J., ZIJLSTRA A.A., ZURITA A., DRAKE J., FABREGAT J., LENNON D.J., LUCAS P.W., MARTIN E.L., PHILLIPPS S., STEEGHS D., UNRUH Y.C.
	Mon. Not. R. Astron. Soc., 388, 89-104 (2008)
	Initial data release from the INT Photometric Hα Survey of the Northern Galactic Plane (IPHAS).
o	<IPHAS JHHMMSS.ss+DDMMSS.s> N~200 million.
Ref:	=2014MNRAS.444.3230B
by	BARENTSEN G. , FARNHILL H.J., DREW J.E., GONZALEZ-SOLARES E.A., GREIMEL R., IRWIN M.J., MISZALSKI B., RUHLAND C., GROOT P., MAMPASO A., SALE S.E., HENDEN A.A., AUNGWEROJWIT A., BARLOW M.J., CARTER P.J., CORRADI R.L.M., DRAKE J.J., EISLOFFEL J., FABREGAT J., GANSICKE B.T., GENTILE FUSILLO N.P., GREISS S., HALES A.S., HODGKIN S., HUCKVALE L., IRWIN J., KING R., KNIGGE C., KUPFER T., LAGADEC E., LENNON D.J., LEWIS J.R., MOHR-SMITH M., MORRIS R.A.H., NAYLOR T., PARKER Q.A., PHILLIPPS S., PYRZAS S., RADDI R., ROELOFS G.H.A., RODRIGUEZ-GIL P., SABIN L., SCARINGI S., STEEGHS D., SUSO J., TATA R., UNRUH Y.C., VAN ROESTEL J., VIIRONEN K., VINK J.S., WALTON N.A., WRIGHT N.J., ZIJLSTRA A.A.
	Mon. Not. R. Astron. Soc., 444, 3230-3257 (2014)
	The second data release of the INT Photometric Hα Survey of the Northern Galactic Plane (IPHAS DR2).
o	<IPHAS JHHMMSS.ss+DDMMSS.s> N=218991524.
=E=	Catalogue in electronic form as <II/321/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: IPHASX
IPHASX	(INT/WFC Photometric H-alpha Survey, extended sources)
Write:	<<IPHASX JHHMMSS.s+DDMMSS>>
Object:	Nebula (SIMBAD class: ISM = Interstellar Medium Object)
Note:	Survey of the Northern Galactic Plane over the Galactic latitude range -5<b<+5, using the Wide Field Camera mounted on the Isaac Newton Telescope. Contemporaneous CCD images in 3 filters are obtained: (i) 95A wide H-alpha filter, (ii) Sloan r, (iii) Sloan i. The data reach down to r=20, approximately. website at: http://astro.ic.ac.uk/Research/Halpha/North/index.html First ref. with an IPHASX object: 2006A&A...458..203M. See also IPHAS, UVEX.
Ref:	=2006A&A...458..203M
by	MAMPASO A. , CORRADI R.L.M., VIIRONEN K., LEISY P., GREIMEL R., DREW J.E., BARLOW M.J., FREW D.J., IRWIN J., MORRIS R.A.H., PARKER Q.A., PHILLIPPS S., RODRIGUEZ-FLORES E.R., ZIJLSTRA A.A.
	Astron. Astrophys., 458, 203-212 (2006)
	The ``Principes de Asturias'' nebula: a new quadrupolar planetary nebula from the IPHAS survey.
o	Text: <IPHASX JHHMMSS.s+DDMMSS> N=1.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: IPN
IPN	(Intracluster PN)
*****	Avoid the usage of IPN, prefer [AGO2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IPS
IPS	(InterPlanetary Scintillation) (Not yet in Simbad)
*****	Avoid the usage of IPS, prefer [PTR87]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IPS
IPS	(InterPlanetary Scintillation)
*****	Avoid the usage of IPS, prefer [ATI98]
Origin	of the Acronym: L (2003A&A...403..555A)
Details on Acronym: [IPS2016]
[IPS2016]	(Iovino+Petropoulou+Scodeggio+, 2016)
Write:	<<[IPS2016] WNN>>
N:	26
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	A galaxy group catalog in the COSMOS field. Use of zCOSMOS VLT VIMOS data. See also [KLI2009] and [KLI2012].
in source:	NAME COSMOS Field
Ref:	=2016A&A...592A..78I
by	IOVINO A. , PETROPOULOU V., SCODEGGIO M., BOLZONELLA M., ZAMORANI G., BARDELLI S., CUCCIATI O., POZZETTI L., TASCA L., VERGANI D., ZUCCA E., FINOGUENOV A., ILBERT O., TANAKA M., SALVATO M., KOVAC K., CASSATA P.
	Astron. Astrophys., 592A, 78-78 (2016)
	A high definition view of the COSMOS Wall at z~ 0.73.
o	Table 4: <[IPS2016] WNN> (Nos W1-W26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: iPTF
iPTF	(intermediate Palomar Transient Factory)
Write:	<<iPTF YYaaa>>
Object:	Opt. Transient (SIMBAD class: Transient = Transient Event)
Note:	The intermediate Palomar Transient Factory survey is a fully-automated, wide-field survey for the systematic exploration of the optical transient sky. More information available at http://ptf.caltech.edu/iptf/ Only the first references are given here. See also PTF.
Ref:	=2013ApJ...775L...7C
by	CAO Y. , KASLIWAL M.M., ARCAVI I., HORESH A., HANCOCK P., VALENTI S., CENKO S.B., KULKARNI S.R., GAL-YAM A., GORBIKOV E., OFEK E.O., SAND D., YARON O., GRAHAM M., SILVERMAN J.M., WHEELER J.C., MARION G.H., WALKER E.S., MAZZALI P., HOWELL D.A., LI K.L., KONG A.K.H., BLOOM J.S., NUGENT P.E., SURACE J., MASCI F., CARPENTER J., DEGENAAR N., GELINO C.R.
	Astrophys. J., 775L, 7 (2013)
	Discovery, progenitor and early evolution of a stripped envelope supernova iPTF13bvn.
o	<iPTF YYaaa> (No. 13bvn).
Ref:	=2013ApJ...776L..34S
by	SINGER L.P. , CENKO S.B., KASLIWAL M.M., PERLEY D.A., OFEK E.O., BROWN D.A., NUGENT P.E., KULKARNI S.R., CORSI A., FRAIL D.A., BELLM E., MULCHAEY J., ARCAVI I., BARLOW T., BLOOM J.S., CAO Y., GEHRELS N., HORESH A., MASCI F.J., McENERY J., RAU A., SURACE J.A., YARON O.
	Astrophys. J., 776L, 34 (2013)
	Discovery and redshift of an optical afterglow in 71 °^{2}: iPTF13bxl and GRB 130702A.
o	<iPTF YYaaa> N=6.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IR
IR	(IR Source) (Not yet in Simbad)
*****	Avoid the usage of IR, prefer [OMD2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IR
IR	(IR Source)
*****	Avoid the usage of IR, prefer [CNK98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ir
ir	(Infrared)
*****	Avoid the usage of ir, prefer [GT89]
Origin	of the Acronym: L (1996ApJS..106..447M)
Details on Acronym: IR
IR	(IR Source)
*****	Avoid the usage of IR, prefer [IBK96]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IR
IR	(IR Source)
*****	Avoid the usage of IR, prefer [JGD88]
Origin	of the Acronym: L (1991PASP..103..487T)
Details on Acronym: IR
IR	(IR Source)
*****	Avoid the usage of IR, prefer [NCG85]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IR
IR	(IR Source)
*****	Avoid the usage of IR, prefer [PCS2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Ir-Ch
Ir-Ch	(Iriarte+Chavira)
*****	Avoid the usage of Ir-Ch, prefer [IC56]
Details on Acronym: IRAC
IRAC	(Infrared Array Camera survey) (Not yet in Simbad)
*****	Avoid the usage of IRAC, prefer [ZWZ2010]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRAC
IRAC	(Infrared Array Camera survey)
*****	Avoid the usage of IRAC, prefer [ALM2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRAC
IRAC	(Infrared Array Camera survey)
*****	Avoid the usage of IRAC, prefer [BBA2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRAC
IRAC	(Infrared Array Camera survey)
*****	Avoid the usage of IRAC, prefer [EBG2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRAC
IRAC	(Infrared Array Camera survey)
*****	Avoid the usage of IRAC, prefer [ESB2004]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRAC
IRAC	(Infrared Array Camera survey)
*****	Avoid the usage of IRAC, prefer [GHB2007]
Origin	of the Acronym: L (2008ApJ...687..406C)
Details on Acronym: IRAC
IRAC	(Infrared Array Camera survey)
*****	Avoid the usage of IRAC, prefer [RRB2009]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRAC
IRAC	(Infrared Array Camera survey)
*****	Avoid the usage of IRAC, prefer [SEB2005]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRAC
IRAC	(Stern+Kirkpatrick+Allen+, 2007)
*****	Avoid the usage of IRAC, prefer [SKA2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRAS
IRAS	(InfraRed Source)
*****	Avoid the usage of IRAS, prefer [ADM95]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRAS
IRAS	(InfraRed source)
*****	Avoid the usage of IRAS, prefer BBH
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRAS
IRAS	(InfraRed source)
*****	Avoid the usage of IRAS, prefer [CTF93]
Origin	of the Acronym: L (2003AJ....126.1916P)
Details on Acronym: IRAS
IRAS	(Infrared Astronomical Satellite)
Write:	<<IRAS HHMM+DDdPNN>>
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Provisory lists have been published as Circulars in Astr. Astrophys. with the format 'HHMM+DDdPNN' where P stands for preliminary and NN is the No. of the Circular. No. 1 : Astr. Astrophys. 123 , C1-C2 , 1983, (N = 18). No. 2 : Astr. Astrophys. 124 , C1-C2 , 1983, (N = 38). No. 3 : Astr. Astrophys. 127 , C1 , 1983, (N = 43). No. 4 : Astr. Astrophys. 128 , C1 , 1983, (N = 20). No. 5 : Astr. Astrophys. 130 , C1 , 1983, (N = 25). No. 6 : Astr. Astrophys. 131 , C1 , 1983, (N = 76). No. 7 : Astr. Astrophys. 131 , C2 , 1983, (N = 28). No. 8 : Astr. Astrophys. 132 , C1 , 1984, (N = 28). No. 9 : Astr. Astrophys. 132 , C2 , 1984, (N = 33). No. 10 : Astr. Astrophys. 134 , C1-C4 , 1984, N = 179, Minisurvey. No. 11 : Astr. Astrophys. 134 , C5 , 1984, (N = 54). No. 12 : (unpublished, contains no sources). No. 13 : Astr. Astrophys. 137 , C1 , 1984, (N = 18). No. 14 : Astr. Astrophys. 137 , C3 , 1984, (N = 24). No. 15 : Astr. Astrophys. 137 , C4 , 1984, (N = 34)
Details on Acronym: IRAS
IRAS	(Infrared Astronomical Satellite)= FSS = LRS = PSC = SSC = SSSC
Write:	<<IRAS HHMMm+DDMMA>> <<IRAS RHHMMm+DDMM>> <<IRAS FHHMMm+DDMMA>> <<IRAS ZHHMMm+DDMM>> <<IRAS SHHMMm+DDMMA>> <<IRAS XHHMM+DDd>>
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat.	in SIMBAD: only PSC
Note:	IRAS catalogues have a catalogue name (see synonyms). IRAS PSC or IRAS P, format HHMMm+DDMMA, and RHHMMm+DDMM for rejected objects. IRAS FSS or IRAS F, format FHHMMm+DDMMA, and ZHHMMm+DDMM for rejected source. (Explanatory Supplement in 1989, Moshir+). IRAS LRS. IRAS SSC or IRAS S, format SHHMMm+DDMMA. IRAS SSSC or IRAS X, format XHHMM+DDdA.
Ref:	=1986SSC...C......0K
by	KLEINMANN S.G. , CUTRI R.M., YOUNG E.T., LOW F.J., GILLETT F.C.
	Tucson, Univ. of Arizona, 0-None (1986)
	IRAS Serendipitous Survey Catalog.
o	<IRAS SHHMMm+DDMMA> N=43886.
Ref:	=1988SSSC..C......0H
by	HELOU G. , WALKER D.W.
	NASA RP-1190, Vol. 7, 0-None (1988)
	Infrared Astronomical Satellite (IRAS), Catalogs and Atlases. Vol. 7. The Small Scale Structure Catalog.
o	<IRAS XHHMM+DDd> N=16740.
Ref:	=1988IRASP.C......0J
by	JOINT IRAS SCIENCE WORKING GROUP
	NASA RP-1190 (1988), 0-None (1988)
	Infrared Astronomical Satellite Catalogs, 1988. The Point Source Catalog, version 2.0, NASA RP-1190.
o	<IRAS HHMMm+DDMMA> N=245889.
Ref:	=1990IRASF.C......0M
by	MOSHIR M. , et al.
	IRAS Faint Source Catalogue, version 2.0, 0-None (1990)
	IRAS Faint Source Catalogue, version 2.0.
o	<IRAS FHHMMm+DDMMA> N=173044.
=E=	Catalogue in electronic form as II/125
=E=	Catalogue in electronic form as II/156
=E=	Catalogue in electronic form as II/126
=E=	Catalogue in electronic form as VII/73
=E=	Catalogue in electronic form as II/274
=E=	Catalogue in electronic form as II/275
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRAS
IRAS	(InfraRed Source)
Write:	<<IRAS CHHMMm+DDMM>>
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	In the format 'CHHMMm+DDMM', C stands for Co-added IRAS sources. Sometimes found as 'IRAS HHMMm+DDMMC'.
Ref:	=1987ApJ...316..311C
by	COHEN M. , SCHWARTZ R.D.
	Astrophys. J., 316, 311-322 (1987)
	IRAS observations of the exciting stars of Herbig-Haro objects.
o	<IRAS CHHMMm+DDMM> N=3.
Ref:	=1991ApJ...370..263S
by	SCHWARTZ R.D. , GYULBUDAGHIAN A.L., WILKING B.A.
	Astrophys. J., 370, 263-271 (1991)
	A search for embedded young stellar objects in and near the IC 1396 complex.
o	Authors use the format HHMMm+DDMMC for Co-added IRAS, but in Simbad use the format CHHMMm+DDMM
o	<IRAS CHHMMm+DDMM> N=20
Ref:	=1995A&A...293...64T
by	TSIKOUDI V. , BROMAGE G.E.
	Astron. Astrophys., 293, 64-68 (1995)
	Far-infrared observations of chromospherically active stars in stellar clusters.
o	<IRAS CHHMMm+DDMM> N=9
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IRAS
IRAS	(InfraRed Source)
*****	Avoid the usage of IRAS, prefer [JCC87]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRAS
IRAS	(InfraRed Source)
*****	Avoid the usage of IRAS, prefer [MLY89]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRAS
IRAS	(InfraRed Source)
*****	Avoid the usage of IRAS, prefer [PC87b]
Origin	of the Acronym: L (1999MNRAS.305..875W)
Details on Acronym: IRAS
IRAS	(InfraRed Source)
*****	Avoid the usage of IRAS, prefer [SHM89]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRAS
IRAS	(InfraRed Source)
*****	Avoid the usage of IRAS, prefer [THL2004]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: iras
iras	(Infrared source)
*****	Avoid the usage of iras, prefer [WGL92]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRAS
IRAS	(InfraRed Source)
*****	Avoid the usage of IRAS, prefer WLY
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRAS-AO
IRAS-AO	(InfraRed Source, Additional Observations)
*****	Avoid the usage of IRAS-AO, prefer IRAS-L
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRAS-L
IRAS-L	(InfraRed Source, Leiden)= (IRAS-AO)
Write:	<<IRAS-L HHMMm+DDMM>>
N:	19+128
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Leiden additional observations of IRAS deep fields.
Ref:	=1988A&A...203..250K
by	KEEL W.C. , DE GRIJP M.H.K., MILEY G.K.
	Astron. Astrophys., 203, 250-254 (1988)
	New active galactic nuclei from the IRAS deep fields.
o	Table 1: <IRAS-L HHMMm+DDMM> N=19.
Ref:	=2005ApJS..158..139K
by	KEEL W.C. , IRBY B.K., MAY A., MILEY G.K., GOLOMBEK D., DE GRIJP M.H.K., GALLIMORE J.F.
	Astrophys. J., Suppl. Ser., 158, 139-160 (2005)
	An atlas of warm active galactic nuclei and starbursts from the IRAS deep fields.
o	Table 1 (si S col. list): IRAS SHHMMm+DDMMA
o	Table 1 (si L col. list): <IRAS-L HHMMm+DDMM> N=128 new. Table 6: <[KIM2005] NN> (Nos 1-31).
=E=	Catalogue in electronic form as J/ApJS/158/139
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRBG
IRBG	(IR-Bright/optically-faint Galaxy)
*****	Avoid the usage of IRBG, prefer [DRA2010]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRC
IRC	(Infrared Catalog)= (TMSS)
Write:	<<IRC +DDNNN>> <<IRC +DD NNN>> (not recognised by Simbad, but found in literature)
N:	about 20000
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	In the format the first two digits (the second is zero) stand for a range in dec: -10 for -15 to -5, n... 0 for -5 to +5 n..., +10 for +5 to +15. The preliminary catalog was published in 1969: NASA SP-3047, Neugebauer + Leighton, Caltech infrared catalog. 1975AJ.....80.1011H: Supplement to the IRC, classifying all unidentified or apparently misidentified IRC sources south of +5deg.
Auth.:	NEUGEBAUER G.+
Ref:	=1969IRC...C......0N
by	NEUGEBAUER G. , LEIGHTON R.B.
	Calif. Inst. Technology, NASA,1969, 0-None (1969)
	Two micron sky survey : A preliminary Catalogue.
o	<IRC +DDNNN> N=5612.
Ref:	=1975AJ.....80.1011H
by	HANSEN O.L. , BLANCO V.M.
	Astron. J., 80, 1011-1025 (1975)
	Classification of 831 two-micron sky survey sources south of +5 °.
o	<IRC +D0NNN> N=551+97+183.
=E=	Catalogue in electronic form as II/2B
Details on Acronym: IRc
IRc	(Infrared compact)
*****	Avoid the usage of IRc, prefer [PF82]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRc
IRc	(Infrared compact)
*****	Avoid the usage of IRc, prefer [RLK73]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRCO
IRCO	(IRAS-CO)
Write:	<<IRCO NNNN>>
N:	4315
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	FCRAO Outer Galactic Survey CO emission and IRAS sources assocation.
Ref:	=2003A&A...399.1083K
by	KERTON C.R. , BRUNT C.M.
	Astron. Astrophys., 399, 1083-1099 (2003)
	The association of IRAS sources and ^{12}CO emission in the outer Galaxy.
o	Table 1: <IRCO NNNN> (Nos 1-4315).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRDC
IRDC	(IR Dark Cloud)
*****	Avoid the usage of IRDC, prefer [AHL2004]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRDC
IRDC	(IR Dark Cloud)
*****	Avoid the usage of IRDC, prefer [BSM2002]
Origin	of the Acronym: L (2005ApJ...634L..57S)
Details on Acronym: IRDC
IRDC	(IR Dark Cloud)
*****	Avoid the usage of IRDC, prefer [CCE98b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRDC
IRDC	(IR Dark Cloud)
*****	Avoid the usage of IRDC, prefer [POR2009]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRDC
IRDC	(IR Dark Cloud)
*****	Avoid the usage of IRDC, prefer [VLH2009]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRe
IRe	(Infrared, extended)
*****	Avoid the usage of IRe, prefer [RLK73]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IREC
IREC	(Infrared Exc. Cloud)= (DBB)
Write:	<<IREC NNN>>
N:	578
Object:	IR Cld (SIMBAD class: Cloud)
Note:	All-Sky map and catalog of significant clouds. Among the 578 clouds, only those outside the galactic plane have been kept in Table 1 (Nos 1-516)
Ref:	=1988ApJ...334..815D
by	DESERT F.X. , BAZELL D., BOULANGER F.
	Astrophys. J., 334, 815-840 (1988)
	An all-sky search for molecular Cirrus clouds.
o	Tables 1,2: <IREC NNN> (Nos 1-516, 559, 570) among 578
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [IRM2004]
[IRM2004]	(Israel+Rea+Mangano+, 2004)
Write:	<<[IRM2004] XN>>
N:	1
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Discovery with the VLT in the IR band of an IR source, proposed as counterpart of XTE J1810-197.
Ref:	=2004ApJ...603L..97I
by	ISRAEL G.L. , REA N., MANGANO V., TESTA V., PERNA R., HUMMEL W., MIGNANI R., AGEORGES N., LO CURTO G., MARCO O., ANGELINI L., CAMPANA S., COVINO S., MARCONI G., MEREGHETTI S., STELLA L.
	Astrophys. J., 603, 97-100 (2004)
	Accurate X-ray position of the anomalous X-ray pulsar XTE J1810-197 and identification of its likely infrared counterpart.
o	Fig.1: <[IRM2004] XN> (No. X1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IRN
IRN	(IR Neb.)
*****	Avoid the usage of IRN, prefer [TGJ91]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRNe
IRNe	(IR Nebula) (Not yet in Simbad)
*****	Avoid the usage of IRNe, prefer [TKK2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRR
IRR	(IR Source)
Note:	Map in Fig. 1
*****	Avoid the usage of IRR, prefer [HDB84]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(International Reference Stars) (Not yet in Simbad)
Write:	<<IRS NNNNN>> <<IRS JHHMMSS.ss+DDMMSS.s>>
N:	36027
Object:	* (SIMBAD class: Star)
Note:	NASA, NSSDC 91-11 (1991), Corbin T.E., Warren W.H. Jr. International Reference Stars (IRS), an all-sky catalog of positions and proper motions that is based on the AGK3R (Corbin 1977, 1978) in the Northern Hemisphere and on the newly completed SRS (Southern Reference Star catalogue, Smith et al. 1990) in the south. (Nos 1-29163) and (70001-76865)
Auth.:	CORBIN T.E.+
=E=	Catalogue in electronic form as I/172
Details on Acronym: IRS
IRS	(IR Source) (Not yet in Simbad)
*****	Avoid the usage of IRS, prefer [B81]
Origin	of the Acronym: L (1989ApJ...345..268B)
Details on Acronym: IRS
IRS	(IR Source) (Not yet in Simbad)
*****	Avoid the usage of IRS, prefer [N2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source) (Not yet in Simbad)
*****	Avoid the usage of IRS, prefer [OTN2004]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: IRS
IRS	(IR Source) (Not yet in Simbad)
*****	Avoid the usage of IRS, prefer [R2009]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(Sato+Tamura+Kandori+, 2008) (Not yet in Simbad)
*****	Avoid the usage of IRS, prefer [STK2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [A72a]
Origin	of the Acronym: L (1972ApL....12..231A)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [AW90]
Origin	of the Acronym: L (1997ApJ...487..346G)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [AWW90]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [B2001b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [B79c]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [BBW79]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [BBW79]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [BC86b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [BCB89]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [BEB76]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [BGD93]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [BJE84]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [C91]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [CHG85]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [CKW92]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
Note:	IR sources near LkHa 198.
*****	Avoid the usage of IRS, prefer [CRB95]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [CS83b]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [CW98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [D77]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [DCL91]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer Dor
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [DS77]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer EB
Origin	of the Acronym: L (1996ApJ...465..363R)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [EC92]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [ELM93]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [FP74]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [FPA77]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [GBM74]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer GCIRS
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [GGC82]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer GWAYL
Origin	of the Acronym: L (2001A&A...372..173B)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [GY92]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [HG83]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [HHS87]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [HKL98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [HPF97]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [HTT95]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [HWJ85]
Origin	of the Acronym: L (2000ApJ...531..861G)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [JMS77]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [KKL96]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [KLT2003]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [KT2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [KWA92]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [LCC2001b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [LDL2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [LHS84]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [LLN92]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer MFSW
Origin	of the Acronym: L = Found in the literature
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [MGL99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [MLG2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [MLH90]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [MRC90]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [MS81]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [P84]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [PCW91]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [PE99b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [PF82]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [PF82]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Irs
Irs	(IR Source)
*****	Avoid the usage of Irs, prefer [PFR86]
Origin	of the Acronym: L (2004AJ....127.2826B)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [PJP92]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [R2007b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [RA2004a]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [RA2004b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [RA2006a]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [RA2006b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [RAB2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [RAL2003]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [RD95]
Origin	of the Acronym: L (2001AJ....121.1556B)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer RRG
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [RW83]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [S87b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [SBH97]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer SBSMH
Origin	of the Acronym: L (2005ApJS..160..379F)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [SDW85]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [SFR97]
Origin	of the Acronym: L (2004ApJ...605..259P)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [SHJ87]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [SHM89]
Origin	of the Acronym: L (2004ApJS..155..123A)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer SSV
Origin	of the Acronym: L = Found in the literature
Details on Acronym: IRS
IRS	(IR Source)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [SVS76]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [T81]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [TEM92]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [TKT2002b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [TRL91]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [TRP85]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [TS84]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [TTH80]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [VMR89]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [W2002]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [WBH2006]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [WBN72]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [WBN74]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [WKM94]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer WLY
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [WMM93]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [WRA93]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [WWH2002]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [WYL99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [WZP2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [YCA2005]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [YCR90]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [YSN87]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [YST88]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRS
IRS	(IR Source)
*****	Avoid the usage of IRS, prefer [ZL78]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRSF
IRSF	(IR Survey Facility)
Write:	<<IRSF JHHMMSSss+DDMMSSs>>
N:	14811185+2769682+434145
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	IRSF 1.4m telescope SIRIUS NIR observations, point sources in the Magellanic Clouds.
in source:	NAME Magellanic Clouds
Ref:	=2007PASJ...59..615K
by	KATO D. , NAGASHIMA C., NAGAYAMA T., KURITA M., KOERWER J.F., KAWAI T., YAMAMURO T., ZENNO T., NISHIYAMA S., BABA D., KADOWAKI R., HABA Y., HATANO H., SHIMIZU H., NISHIMURA M., NAGATA T., SATO S., MURAI Y., KAWAZU T., NAKAJIMA Y., NAKAYA H., KANDORI R., KUSAKABE N., ISHIHARA A., KANEYASU N., HASHIMOTO J., TAMURA M., TANABE T., ITA Y., MATSUNAGA N., NAKADA Y., SUGITANI K., WAKAMATSU K.-I., GLASS I.S., FEAST M.W., MENZIES J.W., WHITELOCK P.A., FOURIE P., STOFFELS J., EVANS G.P., HASEGAWA T.
	PASJ, 59, 615-641 (2007)
	The IRSF Magellanic clouds point source catalog.
o	Catalogue: <IRSF JHHMMSSss+DDMMSSs> N=14811185+2769682+434145.
=E=	Catalogue in electronic form as II/288
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRSN
IRSN	(IR Source, North field) (Not yet in Simbad)
*****	Avoid the usage of IRSN, prefer [RBW98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IRSV
IRSV	(Infrared Survey, Valinhos obs.)
Write:	<<IRSV HHMM+DDMM>>
N:	338
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Ref:	=1985A&AS...61..203E
by	EPCHTEIN N. , MATSUURA O.T., BRAZ M.A., LEPINE J.R.D., PICAZZIO E., MARQUES DOS SANTOS P., BOSCOLO P., LE BERTRE T., ROUSSEL A., TURON P.
	Astron. Astrophys., Suppl. Ser., 61, 203-210 (1985)
	Valinhos 2.2 micron survey of the southern galactic plane. Positions and infrared photometry of 338 sources.
o	Table 1I, col(1): numbering 'NNN' not used.
o	Table I: <IRSV HHMM+DDMM> N=338
Details on Acronym: IRSW
IRSW	(IR Source, West field)
*****	Avoid the usage of IRSW, prefer [RBW98]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [IRW2007]
[IRW2007]	(Indebetouw+Robitaille+Whitney+, 2007)
Write:	<<[IRW2007] HH-W>> <<[IRW2007] P5A>> <<[IRW2007] MYSO>>
N:	2+2+1
Object:	Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC photometry of the Eagle Nebula = M 16. See also [PAB98], [STN2002].
in source:	M 16 = Eagle Nebula = NGC 6611
Ref:	=2007ApJ...666..321I
by	INDEBETOUW R. , ROBITAILLE T.P., WHITNEY B.A., CHURCHWELL E., BABLER B., MEADE M., WATSON C., WOLFIRE M.
	Astrophys. J., 666, 321-338 (2007)
	Embedded star formation in the Eagle nebula with Spitzer GLIMPSE.
o	Table 1: <[IRW2007] HH-W> (Nos HH-N, HH-S), <[IRW2007] P5A> (Nos P5A, P5B), <[IRW2007] MYSO> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Irwin
Irwin	(Irwin)
Write:	<<Irwin UMi NNNNN>> <<Irwin Dra NNNNN>>
Object:	Dw. * (SIMBAD class: Star)
Note:	In the format, 'NNNNN' (always a 5 digit number) stands for the number in Irwin's APM catalog, provided to the authors by M. Irwin, unpublished, here in UMi and Draco dwarf galaxies.
in source:	NAME UMi Dwarf Galaxy
in source:	NAME Draco Dwarf Galaxy
Ref:	=1995AJ....110.2120O
by	OLSZEWSKI E.W. , AARONSON M., HILL J.M.
	Astron. J., 110, 2120-2130 (1995)
	Nine seasons of velocity measurements in the Draco and Ursa minor dwarf spheroidal galaxies with the MMT echelle.
o	Other acronymes used: T1,6: JI = UMJI, COS, CUD = COS, EDO NNN = COS, EDO A = [V67] A, A = [V67] A, VA = [V67], EDON NN = Olsz ANN (letter A=N), ANN (letter A=N) = Olsz ANN. T.2,7: NNN = [BS61] NNN.
o	Tables 1, 6: <Irwin UMi NNNNN>, <Olsz ANN> (letter A = N), <SOK NNNqN>. Tables 2, 7: <Irwin Dra NNNNN>, <McClure R-NN> and <McClure CN> (Nos C1-C4), <Stetson Draco NNNN>.
Ref:	=1995AJ....110.2131A
by	ARMANDROFF T.E. , OLSZEWSKI E.W., PRYOR C.
	Astron. J., 110, 2131-2165 (1995)
	The mass-to-light ratios of the Draco and Ursa minor dwarf spheroidal galaxies. I. Radial velocities from multifiber spectroscopy.
o	Other acronyms used: T.2,4: JI = UMJI, COS, CUD = COS, EDO NNN = COS, EDO A = [V67] A, A = [V67] A, VA = [V67], EDON NN = Olsz ANN (letter A=N), ANN (letter A=N) = Olsz ANN, T.3,5: NNN, A = [BS61] NNN, [BS61] A.
o	Tables 2, 4: <Irwin UMi NNNNN>, <Olsz ANN>, <SOK NNNqN>, Tables 3, 5: <Irwin Dra NNNNN>, <McClure R-NN> and <McClure CN> (Nos C1-C4), <Stetson NNNN>.
=E=	Catalogue in electronic form as J/AJ/110/2131
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IRXS
IRXS	(IR Excess source)
Write:	<<IRXS GLLL.l+B.b>>
N:	16
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Use of IRAS, CGPS, and FCRAO Outer Galaxy Survey data to search for IR Excess sources.
Ref:	=2007ApJ...659..426D
by	DOUGLAS K.A. , TAYLOR A.R.
	Astrophys. J., 659, 426-440 (2007)
	Infrared excess sources in the Canadian Galactic Plane Survey.
o	Table 2: <IRXS GLLL.l+B.b> N=16.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IS
IS	(Irwin+Seaquist)
*****	Avoid the usage of IS, prefer [IS88]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [IS2012]
[IS2012]	(Il'ina+Sil'chenko O.k, 2012) (Not yet in Simbad)
Write:	<<[IS2012] NGC NNN NN>>
N:	97
Object:	G (SIMBAD class: Galaxy)
Notes:	SAO 6m telescope SCORPIO photometric observations of N=12+22+14+13+12+24 dwarf galaxies of the NGC 524 group of galaxies.
in source:	NAME NGC 524 Group
in source:	NGC 502
in source:	NGC 509
in source:	NGC 516
in source:	NGC 518
in source:	NGC 524
in source:	NGC 532
Ref:	=2012ARep...56..578I
by	IL'INA M.A. , SIL'CHENKO O.K.
	ARep, 56, 578-588 (2012)
	Structural analysis of disk galaxies of the NGC 524 group.
o	2012AZh....89..640I
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IS73]
[IS73]	(Isserstedt+Schmidt-Kaler, 1973)
Write:	<<[IS73] 2-NNN>> <<[IS73] 3-NNN>>
N:	207+267
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Photometry of a star field within OB aggregate Mon OB 1, centered on the open cluster Collinder 107 and containing a stellar ring.
in source:	NAME ASS MON OB 1-
Ref:	=1973A&AS...10..365I
by	ISSERSTEDT J. , SCHMIDT-KALER T.
	Astron. Astrophys., Suppl. Ser., 10, 365-383 (1973)
	Der offene Sternhaufen Collinder 107 und ein Sternring in Monoceros.
o	Table 2: <[IS73] 2-NNN> (Nos 2-1 to 2-207). Table 3: <[IS73] 3-NNN> (Nos 3-1 to 3-267).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IS88]
[IS88]	(Irwin+Seaquist, 1988)= (IS)
Write:	<<[IS88] A>>
N:	6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLBI observations of the nuclear region of NGC 3079. N=6 radio-components of NGC 3079. D = Dynamical centre, E and F are 18-cm components from Middleberg et al (2003). Map in Fig.2 of 1srt ref.
in source:	NGC 3079
Ref:	=1988ApJ...335..658I
by	IRWIN J.A. , SEAQUIST E.R.
	Astrophys. J., 335, 658-667 (1988)
	Nuclear jets in the radio lobe spiral galaxy, NGC 3079.
o	Table 2: <[IS88] A> (Nos A-C)
Ref:	=1998ApJ...495..740T
by	TROTTER A.S. , GREENHILL L.J., MORAN J.M., REID M.J., IRWIN J.A., LO K.-Y.
	Astrophys. J., 495, 740-748 (1998)
	Water maser emission and the parsec-scale jet in NGC 3079.
o	Water maser = [CPF88] 095835.0+555517.6
o	Table 2: <[IS88] A> (No. D) added.
Ref:	=2004MNRAS.353.1055H
by	HAGIWARA Y. , KLOECKNER H.-R., BAAN W.
	Mon. Not. R. Astron. Soc., 353, 1055-1063 (2004)
	VLBI imaging of OH absorption: the puzzle of the nuclear region of NGC3079.
o	Fig.7: <[IS88] A> (Nos E-F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IS94]
[IS94]	(Indrani+Sridharan, 1994)
Write:	<<[IS94] NN>>
N:	21
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
in source:	NAME ASS CEP OB 2-
Ref:	=1994JApA...15..157I
by	INDRANI C. , SRIDHARAN T.K.
	J. Astrophys. Astron., 15, 157-163 (1994)
	Observations of the bright-rimmed molecular clouds near the Cepheus OB 2 association.
o	<[IS94] NN> N=21
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IS95]
[IS95]	(Irwin+Sarazin, 1995)
Write:	<<[IS95] NN>>
N:	24
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC and HRI observations of 2A 0335+096 cluster.
in source:	2A 0335+096
Ref:	=1995ApJ...455..497I
by	IRWIN J.A. , SARAZIN C.L.
	Astrophys. J., 455, 497-507 (1995)
	ROSAT X-ray observations of the 2A 0335+096 cluster of galaxies.
o	NAME CENTRAL D GALAXY = [SBO95] 1
o	Table 1: <[IS95] NN> (Nos 1-24)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ISA2022]
[ISA2022]	(Inami+Surace+Armus+, 2022)
Write:	<<[ISA2022] NN>>
N:	12
Object:	(MIR) + Clump (SIMBAD class: PartofG = Part of a Galaxy)
Stat:	is completely incorporated in Simbad
Note:	JWST MIRI observations of N=12 clumps in Zw II 96.
in source:	IRAS 20550+1656 = Zw II 96
Ref:	=2022ApJ...940L...6I
by	INAMI H. , SURACE J., ARMUS L., EVANS A.S., LARSON K.L., BARCOS-MUNOZ L., STIERWALT S., MAZZARELLA J.M., PRIVON G.C., SONG Y., LINDEN S.T., HAYWARD C.C., BOKER T., U V., BOHN T., CHARMANDARIS V., DIAZ-SANTOS T., HOWELL J.H., LAI T., MEDLING A.M., RICH J.A., AALTO S., APPLETON P., BROWN M.J.I., HOSHIOKA S., IWASAWA K., KEMPER F., LAW D., MALKAN M.A., MARSHALL J., MURPHY E.J., SANDERS D., VAN DER WERF P.
	Astrophys. J., 940L, 6 (2022)
	GOALS-JWST: Unveiling Dusty Compact Sources in the Merging Galaxy IIZw096.
o	Fig. 1, Table 1: <[ISA2022] NN> (Nos 1-12).
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [ISA97]
[ISA97]	(Israel+Stella+Angelini+, 1997)
Write:	<<[ISA97] Star N>>
N:	1
Object:	* (SIMBAD class: Star)
Note:	N=1 previously unclassified star in the field of 2E 0050.1-7247.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1997ApJ...484L.141I
by	ISRAEL G.L. , STELLA L., ANGELINI L., WHITE N.E., GIOMMI P., COVINO S.
	Astrophys. J., 484, 141-144 (1997)
	The discovery of 8.9 second pulsations from the variable X-ray source 2E 0050.1-7247 in the Small Magellanic Cloud.
o	<[ISA97] Star N> (No. 1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ISB2000]
[ISB2000]	(Irwin+Sarazin+Bregman, 2000)
Write:	<<[ISB2000] NN>>
N:	12
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT PSPC and ASCA data of NGC 4697. See also [SIB2001].
in source:	NGC 4697
Ref:	=2000ApJ...544..293I
by	IRWIN J.A. , SARAZIN C.L., BREGMAN J.N.
	Astrophys. J., 544, 293-301 (2000)
	The X-ray-faint early-type galaxy NGC 4697.
o	Table 1: <[ISB2000] NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ISB2002]
[ISB2002]	(Irwin+Sarazin+Bregman, 2002)
Write:	<<[ISB2002] NN>>
N:	48
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-S observations of NGC 1291.
in source:	NGC 1291
Ref:	=2002ApJ...570..152I
by	IRWIN J.A. , SARAZIN C.L., BREGMAN J.N.
	Astrophys. J., 570, 152-164 (2002)
	Untangling the X-ray emission from the Sa galaxy NGC 1291 with Chandra.
o	Table 1: <[ISB2002] NN> (Nos 1-48).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ISC99]
[ISC99]	(Israel+Stella+Covino+, 1999)
Write:	<<[ISC99] JHHMMSS.s+DDMMSS>>
N:	3
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	'J005214.0-731918' is a B star, likely optical counterpart of RX J0052.1-7319. The 2 other stars are in the error circle of XTE J0111-732.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1999IAUC.7101Q...1I
by	ISRAEL G.L. , STELLA L., COVINO S., CAMPANA S., MEREGHETTI S.
	IAU Circ., 7101, 1-None (1999)
	RX J0052.1-7319 and XTE J0111.2-7317.
o	<[ISC99] JHHMMSS.s+DDMMSS> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ISCS
ISCS	(IRAC Shallow Cluster Search)
Write:	<<ISCS JHHMMSS+DDMMSS>> <<ISCS JHHMM.m+DDMM>>
N:	1+12+8
Object:	Cl of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	Spitzer IRAC Shallow survey Cluster Search: First refs with ISCS cluster. See also [SEB2005], [EBG2008], [ZSB2013], for galaxies in ISCS clusters.
Ref:	=2005ApJ...634L.129S
by	STANFORD S.A. , EISENHARDT P.R., BRODWIN M., GONZALEZ A.H., STERN D., JANNUZI B.T., DEY A., BROWN M.J.I., McKENZIE E., ELSTON R.
	Astrophys. J., 634, 129-132 (2005)
	An IR-selected galaxy cluster at z = 1.41.
o	Text: <ISCS JHHMMSS+DDMMSS> N=1. Table 1: <[SEB2005] IRAC JHHMMSS+DDMMSS> N=5.
Ref:	=2008ApJ...684..905E
by	EISENHARDT P.R.M. , BRODWIN M., GONZALEZ A.H., STANFORD S.A., STERN D., BARMBY P., BROWN M.J.I., DAWSON K., DEY A., DOI M., GALAMETZ A., JANNUZI B.T., KOCHANEK C.S., MEYERS J., MOROKUMA T., MOUSTAKAS L.A.
	Astrophys. J., 684, 905-932 (2008)
	Clusters of galaxies in the first half of the universe from the IRAC Shallow Survey.
o	Table 1: <ISCS JHHMM.m+DDMM> N=12. Table 3: <[EBG2008] IRAC JHHMMSS.s+DDMMSS> N=97, <[EBG2008] ser JHHMMSS.s+DDMMSS> N=7.
Ref:	=2013ApJ...779..137Z
by	ZEIMANN G.R. , STANFORD S.A., BRODWIN M., GONZALEZ A.H., MANCONE C., SNYDER G.F., STERN D., EISENHARDT P., DEY A., MOUSTAKAS J.
	Astrophys. J., 779, 137 (2013)
	Hα star formation rates of z > 1 galaxy clusters in the IRAC Shallow Cluster Survey.
o	Table 1: <ISCS JHHMM.m+DDMM> N=8 added. Table 2: <[ZSB2013] JHHMMSS.s+DDMMSS> N=459.
=E=	Catalogue in electronic form as <J/ApJ/684/905/>
=E=	Catalogue in electronic form as <J/ApJ/779/137/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ISF2001]
[ISF2001]	(Ivison+Smail+Frayer+, 2001)
Write:	<<[ISF2001] ACO 1835 J1n>>
N:	1
Object:	Knot (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST observations. N=1 bright object, diffuse and very red component north of the galaxy [BCS99b] ACO 1835 J1. See [BCS99b].
in source:	ACO 1835:[BCS99b] ACO 1835 J1 = [BCS99b] ACO 1835 J1
Ref:	=2001ApJ...561L..45I
by	IVISON R.J. , SMAIL I., FRAYER D.T., KNEIB J.-P., BLAIN A.W.
	Astrophys. J., 561, 45-49 (2001)
	Locating the starburst in the SCUBA galaxy SMM J14011+0252.
o	Fig.1: <[ISF2001] ACO 1835 J1n> = <[BCS99b] ACO 1835 J1n> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ISF2002]
[ISF2002]	(Im+Simard+Faber+, 2002)
Write:	<<[ISF2002] FFN-xxyy>>
N:	145
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	DEEP Groth Strip survey: (Groth Strip is a mosaic of 28 fields) N=145 E/S0 galaxies are observed. Format 'FFC-xxyy', see DEEP-GSS.
Ref:	=2002ApJ...571..136I
by	IM M. , SIMARD L., FABER S.M., KOO D.C., GEBHARDT K., WILLMER C.N.A., PHILLIPS A., ILLINGWORTH G., VOGT N.P., SARAJEDINI V.L.
	Astrophys. J., 571, 136-171 (2002)
	The DEEP Groth Strip survey. X. Number density and luminosity function of field E/S0 galaxies at z < 1.
o	Table 2: <[ISF2002] NNN-NNNN> N=145.
=E=	Catalogue in electronic form as J/ApJ/571/136
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ISG
ISG	(Isserstedt+Schindler, G)
Write:	<<ISG NN>>
N:	59
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Ref:	=1986A&A...167...11I
by	ISSERSTEDT J. , SCHINDLER R.
	Astron. Astrophys., 167, 11-24 (1986)
	Spate Galaxien. Die Sternentstehungsraten.
o	Table 1: <ISG NN> (Nos 1-59)
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [ISG2004]
[ISG2004]	(Iyer+Simpson+Gottesman+, 2004) (Not yet in Simbad)
Write:	<<[ISG2004] A>>
N:	3
Object:	HI (SIMBAD class: HI = HI (21cm) Source)
Note:	N=3 HI concentration regions in APG 158.
in source:	APG 158
Ref:	=2004AJ....128..985I
by	IYER M.G. , SIMPSON C.E., GOTTESMAN S.T., MALPHRUS B.K.
	Astron. J., 128, 985-996 (2004)
	Neutral hydrogen in Arp 158.
o	Table 1, Fig.2: <[ISG2004] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ISI
ISI	(Impey+Sprayberry+Irwing+)
*****	Avoid the usage of ISI, prefer ISI96
Origin	of the Acronym: L (2002ApJS..141..123W)
Details on Acronym: ISI96
ISI96	(Impey+Sprayberry+Irwing+, 1996)= (ISI) = LSBG
Write:	<<ISI96 HHMM+DDMMa>>
N:	692
Object:	G (SIMBAD class: LowSurfBrghtG = Low Surface Brightness Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Catalogue of LSBG: N=693 galaxies identified from the UKST survey plates.
Ref:	=1996ApJS..105..209I
by	IMPEY C.D. , SPRAYBERRY D., IRWIN M.J., BOTHUN G.D.
	Astrophys. J., Suppl. Ser., 105, 209-267 (1996)
	Low surface brightness galaxies in the local universe. I. The catalog.
o	Tables 1, 2: <ISI96 HHMM+DDMMa> N=693.
=E=	Catalogue in electronic form as J/ApJS/105/209
Origin	of the Acronym: L (1999A&AS..135..221K)
Details on Acronym: ISIB
ISIB	(Impey+Sprayberry+Irwing+Bothun)
*****	Avoid the usage of ISIB, prefer ISI96
Origin	of the Acronym: L (2004MNRAS.349..576C)
Details on Acronym: [ISK2007]
[ISK2007]	(Ikeda+Sunada+Kitamura, 2007)
Write:	<<[ISK2007] NNN>>
N:	236
Object:	H13CO+ core (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	Nobeyama 45m telescope observations of the Ori A Cloud.
in source:	NAME Ori A
Ref:	=2007ApJ...665.1194I
by	IKEDA N. , SUNADA K., KITAMURA Y.
	Astrophys. J., 665, 1194-1219 (2007)
	A survey of dense cores in the Orion A cloud.
o	Table 1: <[ISK2007] NNN> (Nos 1-236).
=E=	Catalogue in electronic form as J/ApJ/665/1194
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Iskudarian
Iskudarian	(Iskudarian)
*****	Avoid the usage of Iskudarian, prefer Iskurzdajan
Details on Acronym: Iskurzdajan
Iskurzdajan	(Iskudarian)= (Iskudarian)
Write:	<<Cl Iskurzdajan N>>
N:	1
Object:	OCl (SIMBAD class: OpenCluster = Open Cluster)
Stat:	is completely incorporated in Simbad
Ref:	=1961ATsir.221....6I
by	ISKUDARIAN S.G. , SAAKIAN K.A.
	Astron. Tsirk., 221, 6-9 (1961)
	The cluster of white dwarfs in Lyrae.
o	<Cl Iskurzdajan N> (No. 1).
Details on Acronym: [ISL98]
[ISL98]	(Ivison+Smail+Le Borgne+, 1998)
Write:	<<[ISL98] LN>> <<[ISL98] LNWW>>
N:	3+2
Object:	Poss. Opt. Counterpart + Dark Cloud (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=2 possible optical counterparts to [BCS98] SMM J02399-0136. N=1 dark cloud, a luminous Lyα emitter.
in source:	ACO 370
Ref:	=1998MNRAS.298..583I
by	IVISON R.J. , SMAIL I., LE BORGNE J.-F., BLAIN A.W., BEZECOURT J., KERR T.H., DAVIES J.K.
	Mon. Not. R. Astron. Soc., 298, 583-593 (1998)
	A hyperluminous galaxy at z = 2.8 found in a deep submillimetre survey.
o	Table I: <[ISL98] LN> (Nos L1-L2).
Ref:	=2010MNRAS.404..198I
by	IVISON R.J. , SMAIL I., PAPADOPOULOS P.P., WOLD I., RICHARD J., SWINBANK A.M., KNEIB J.-P., OWEN F.N.
	Mon. Not. R. Astron. Soc., 404, 198-205 (2010)
	Gas, dust and stars in the SCUBA galaxy, SMMJ02399-0136: the EVLA reveals a colossal galactic nursery.
o	Fig. 1: <[ISL98] LNWW> (Nos L1N, L2SW).
Ref:	=2019ApJ...875..130L
by	LI Q. , CAI Z., PROCHASKA J.X., ARRIGONI BATTAIA F., IVISON R.J., FALGARONE E., CANTALUPO S., MATUSZEWSKI M., NEILL J.D., WANG R., MARTIN C., MOORE A.
	Astrophys. J., 875, 130-130 (2019)
	Discovery of a Lyα-emitting dark cloud within the z ~ 2.8 SMM J02399-0136 system.
o	Fig. 1, Table 1: <[ISL98] LN> (No. L3) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ISM2001]
[ISM2001]	(Ishwara-Chandra+Saikia+McCarthy+, 2001)
Write:	<<[ISM2001] MRC 0428-281 Galaxy A>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	N=2 galaxies in the field of MRC 0428-281.
Ref:	=2001MNRAS.323..460I
by	ISHWARA-CHANDRA C.H. , SAIKIA D.J., McCARTHY P.J., VAN BREUGEL W.J.M.
	Mon. Not. R. Astron. Soc., 323, 460-470 (2001)
	A radio and optical study of Molonglo radio sources.
o	Fig.7: <[ISM2001] MRC 0428-281 Galaxy A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ISM2017]
[ISM2017]	(Imai+Sugitani+Miao+, 2017)
Write:	<<[ISM2017] SNa>> <<[ISM2017] N>>
N:	10+3
Object:	YSO + Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Stat:	is completely incorporated in Simbad
Note:	UH88 (optical and NIR) and Subaru CIAO (NIR) observations of N=10 YSOs and N=3 YSO candidates toward SFO 12. Use of archival Spitzer, Herschel, and JCMT data.
in source:	SFO 12
in source:	NAME IRAS 02511+6023 Stellar Group
Ref:	=2017ApJ...845...99I
by	IMAI R. , SUGITANI K., MIAO J., FUKUDA N., WATANABE M., KUSUNE T., PICKLES A.J.
	Astrophys. J., 845, 99-99 (2017)
	High-resolution near-infrared observations of a small cluster associated with a bright-rimmed cloud in W5.
o	Table 2: Sources S2a, S2b, S3a and S3b are not in SIMBAD (no coordinates)
o	Fig. 3, Tables 1-2: <[ISM2017] SNa> (Nos S1-S2, S2a-S2b, S3, S3a-S3b, S4-S6). Fig. 2, Table 3: <[ISM2017] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ISN2011]
[ISN2011]	(Ibata+Sollima+Nipoti+, 2011)
Write:	<<[ISN2011] NNN>>
N:	178
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Keck II DEIMOS spectroscopy of the globular cluster NGC 2419. Use of HST ACS photometry and Subaru Suprime-Cam data.
in source:	NGC 2419
Ref:	=2011ApJ...738..186I
by	IBATA R. , SOLLIMA A., NIPOTI C., BELLAZZINI M., CHAPMAN S.C., DALESSANDRO E.
	Astrophys. J., 738, 186 (2011)
	The globular cluster NGC 2419: a crucible for theories of gravity.
o	Table 3: <[ISN2011] NNN> (Nos 1-178).
=E=	Catalogue in electronic form as J/ApJ/738/186
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ISO
ISO	(Infrared Source Obs.) (Not yet in Simbad)
*****	Avoid the usage of ISO, prefer [FHD99]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ISO
ISO	(ISO, Cha I)
====>	Equivalent to: ISO-ChaI
Origin	of the Acronym: L = Found in the literature
Details on Acronym: ISO
ISO	(ISO, Cha II)
====>	Equivalent to: ISO-ChaII
Origin	of the Acronym: L = Found in the literature
Details on Acronym: ISO
ISO	(Infrared Source Obs.)
*****	Avoid the usage of ISO, prefer ISO-Oph
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ISO
ISO	(ISOCAM)
*****	Avoid the usage of ISO, prefer [KOB2004]
Origin	of the Acronym: L (2005AJ....130..643E)
Details on Acronym: ISO
ISO	(Infrared Source Obs.)
*****	Avoid the usage of ISO, prefer [OSP2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ISO
ISO	(Infrared Source Obs.)
*****	Avoid the usage of ISO, prefer [PLH2001]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ISO-ChaI
ISO-ChaI	(ISO, Cha I)= (ISO)
Write:	<<ISO-ChaI NNN>>
N:	105
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	ISOCAM sources.
in source:	NAME Cha I
Ref:	=2000A&A...357..219P
by	PERSI P. , MARENZI A.R., OLOFSSON G., KAAS A.A., NORDH L., HULDTGREN M., ABERGEL A., ANDRE P., BONTEMPS S., BOULANGER F., BURGDORF M., CASALI M.M., CESARSKY C.J., COPET E., DAVIES J., FALGARONE E., MONTMERLE T., PERAULT M., PRUSTI T., PUGET J.L., SIBILLE F.
	Astron. Astrophys., 357, 219-224 (2000)
	ISOCAM observations of the Chamaeleon I dark cloud.
o	Tables 1-4: <ISO-ChaI NNN> N=105 among (Nos 1-282).
=E=	Catalogue in electronic form as J/A+A/357/219
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ISO-ChaII
ISO-ChaII	(ISO, Cha II)= (ISO)
Write:	<<ISO-ChaII NNN>>
N:	115
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	ISOCAM sources. See also [PMG2003].
in source:	NAME Cha II
Ref:	=2003A&A...399..995P
by	PERSI P. , MARENZI A.R., GOMEZ M., OLOFSSON G.
	Astron. Astrophys., 399, 995-1002 (2003)
	Near-infrared and ISOCAM observations of the Chamaeleon II dark cloud.
o	in table 1, YHX98 not found.
o	Table 1: <ISO-ChaII NNN> (Nos 1-115). Table 2: <[PMG2003] NIR NNN> (Nos 1-197).
=E=	Catalogue in electronic form as J/A+A/399/995
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ISO-Cl0024
ISO-Cl0024	(ISOCAM survey, ClG 0024+1654)
Write:	<<ISO-Cl0024 NN>> <<ISO-Cl0024 Ns>>
N:	30+5
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	ISOCAM observations of ClG 0024+1654.
in source:	ClG 0024+1652 = HMS 0024+1654
Ref:	=2005A&A...431..433C
by	COIA D. , McBREEN B., METCALFE L., BIVIANO A., ALTIERI B., OTT S., FORT B., KNEIB J.-P., MELLIER Y., MIVILLE-DESCHENES M.-A., O'HALLORAN B., SANCHEZ-FERNANDEZ C.
	Astron. Astrophys., 431, 433-449 (2005)
	An ISOCAM survey through gravitationally lensing galaxy clusters. IV. Luminous infrared galaxies in Cl 0024+1654 and the dynamical status of clusters.
o	Table 2: <ISO-Cl0024 NN> (Nos 1-30). Table 3: <ISO-Cl0024 Ns> (Nos 1s-5s).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ISO-CrA
ISO-CrA	(ISO, CrA)
Write:	<<ISO-CrA NNN>>
N:	31
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	ISOCAM sources.
in source:	NAME CrA Complex
Ref:	=1999A&A...350..883O
by	OLOFSSON G. , HULDTGREN M., KAAS A.A., BONTEMPS S., NORDH L., ABERGEL A., ANDRE P., BOULANGER F., BURGDORF M., CASALI M.M., CESARSKY C.J., DAVIES J., FALGARONE E., MONTMERLE T., PERAULT M., PERSI P., PRUSTI T., PUGET J.L., SIBILLE F.
	Astron. Astrophys., 350, 883-890 (1999)
	ISOCAM observations of the RCrA star formation region.
o	Tables 1, 2: <ISO-CrA NNN> N=31 among 234.
=E=	Catalogue in electronic form as J/A+A/350/883
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ISO-LHDS
ISO-LHDS	(ISOCAM, Lockman Hole Deep Survey)
Write:	<<ISO-LHDS JHHMMSS+DDMMSS>>
N:	283
Object:	* + G (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	ISOCAM 14.3mu.m smaller deeper survey of the Lockman Hole. See also [RLF2004]. See also ISO-LHSS larger shallow survey.
in source:	NAME Lockman Hole
Ref:	=2004A&A...427..773R
by	RODIGHIERO G. , LARI C., FADDA D., FRANCESCHINI A., ELBAZ D., CESARSKY C.
	Astron. Astrophys., 427, 773-783 (2004)
	ISOCAM observations in the Lockman Hole. II. The 14.3 µm deep survey: Data reduction, catalogue and source counts.
o	table2.dat: <[RLF2004] NNN> (Nos 1-283) = <ISO-LHDS JHHMMSS+DDMMSS> N=283.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ISO-LHSS
ISO-LHSS	(ISOCAM, Lockman Hole Shallow Survey)
Write:	<<ISO-LHSS JHHMMSS+DDMMS>>
N:	259+197
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	Image and catalogue of the 14.3mu.m larger shallow survey in the region of the Lockman Hole with the Infrared Space Observatory. See also ISO-LHDS smaller shallow survey.
in source:	NAME Lockman Hole
Ref:	=2004A&A...427...23F
by	FADDA D. , LARI C., RODIGHIERO G., FRANCESCHINI A., ELBAZ D., CESARSKY C., PEREZ-FOURNON I.
	Astron. Astrophys., 427, 23-34 (2004)
	ISOCAM observations in the Lockman Hole. I. The 14.3 µm shallow survey: Data reduction, catalogue, and optical identifications.
o	Unusual truncation of ISO-LHSS: JHHMMSS+DDMMS
o	Table 2: <[FLR2004] JHHMMSS.sss+DDMMSS.ss> N=21. Tables 3, 4: <ISO-LHSS JHHMMSS+DDMMS> N=259+197.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ISO-MCMS
ISO-MCMS	(Infrared Source Obs., Magellanic Clouds Mini-Survey)
Write:	<<ISO-MCMS JHHMMSS.s+DDMMSS>>
N:	458+44
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	ISO Mini-Survey catalogue of the Magellanic Clouds. First objects from the catalogue in 2003A&A...406...51C (study of light curves extracted from the MACHO database for a sample of ISO-MCMS objects).
Ref:	=2003A&A...406...51C
by	CIONI M.-R.L. , BLOMMAERT J.A.D.L., GROENEWEGEN M.A.T., HABING H.J., HRON J., KERSCHBAUM F., LOUP C., OMONT A., VAN LOON J.T., WHITELOCK P.A., ZIJLSTRA A.A.
	Astron. Astrophys., 406, 51-63 (2003)
	Long period variables detected by ISO in the Small Magellanic Cloud.
o	In reflist, Wood and al., 1985 : AJ is a misprint for ApJ.
o	Tables 1, 2, 4: <ISO-MCMS JHHMMSS.s+DDMMSS> N=458+44
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ISO-Oph
ISO-Oph	(ISO, Oph)= (ISO)
Write:	<<ISO-Oph NNN>> <<ISO-Oph NNNa>>
N:	212+11
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	ISOCAM observations of rho Oph Cloud. The IR stars are sometimes multiple: format NNNa.
in source:	NAME rho Oph Cloud
Ref:	=2001A&A...372..173B
by	BONTEMPS S. , ANDRE P., KAAS A.A., NORDH L., OLOFSSON G., HULDTGREN M., ABERGEL A., BLOMMAERT J., BOULANGER F., BURGDORF M., CESARSKY C.J., CESARSKY D., COPET E., DAVIES J., FALGARONE E., LAGACHE G., MONTMERLE T., PERAULT M., PERSI P., PRUSTI T., PUGET J.L., SIBILLE F.
	Astron. Astrophys., 372, 173-194 (2001)
	ISOCAM observations of the ρ Ophiuchi cloud: Luminosity and mass functions of the pre-main sequence embedded cluster.
o	Table 1: <ISO-Oph NNN> (Nos 1-212).
Ref:	=2006A&A...452..245N
by	NATTA A. , TESTI L., RANDICH S.
	Astron. Astrophys., 452, 245-252 (2006)
	Accretion in the ρ-Ophiuchi pre-main sequence stars.
o	Tables C1, C2, C3: <ISO-Oph NNNa> N=11 added.
=E=	Catalogue in electronic form as J/A+A/372/173
=E=	Catalogue in electronic form as J/A+A/452/245
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ISOCP
ISOCP	(ISOCAM Parallel survey)
Write:	<<ISOCP NNNNN>>
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	ISOCAM Parallel survey: 3 ISOCP sources in 2004A&A...419L..49H. See also [HSL2004].
Ref:	=2004A&A...419L..49H
by	HAAS M. , SIEBENMORGEN R., LEIPSKI C., OTT S., CUNOW B., MEUSINGER H., MUELLER S.A.H., CHINI R., SCHARTEL N.
	Astron. Astrophys., 419, 49-53 (2004)
	Mid-infrared selection of AGN.
o	Fig.2: <ISOCP NNNNN> N=3. Text: <[HSL2004] JHHMMSS.s+DDMMSS> N=1
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ISOGAL-P
ISOGAL-P	(ISOGAL, Point Source Catalogue)
Write:	<<ISOGAL-P JHHMMSS.s+DDMMSS>>
N:	106150
Object:	(IR) (SIMBAD class: MidIR = Mid-IR Source (3 to 30 µm))
Note:	ISOGAL-DENIS Point Source Catalogue of sources in the inner galaxy with ISOCAM instrument on board of the Infrared Space Observatory (ISO satellite).
Ref:	=1999MNRAS.308..127G
by	GLASS I.S. , GANESH S., ALARD C., BLOMMAERT J.A.D.L., GILMORE G., LLOYD EVANS T., OMONT A., SCHULTHEIS M., SIMON G.
	Mon. Not. R. Astron. Soc., 308, 127-139 (1999)
	ISOGAL survey of Baade's Windows in the mid-infrared.
o	Notes to Tables 2 and 3: B = stars classified by Blanco, 1986 (not BMB).
o	Table 2: <[GGA99] NGC 6522 NNN> N=33 among 497 = <ISOGAL-P JHHMMSS.s+DDMMSS> N=33. Table 3: <[GGA99] Sgr I NNN> N=64 among 696 = <ISOGAL-P JHHMMSS.s+DDMMSS> N=64.
Ref:	=1999A&A...348..755O
by	OMONT A. , GANESH S., ALARD C., BLOMMAERT J.A.D.L., CAILLAUD B., COPET E., FOUQUE P., GILMORE G., OJHA D., SCHULTHEIS M., SIMON G., BERTOU X., BORSENBERGER J., EPCHTEIN N., GLASS I., GUGLIELMO F., GROENEWEGEN M.A.T., HABING H.J., KIMESWENGER S., MORRIS M., PRICE S.D., ROBIN A., UNAVANE M., WYSE R.
	Astron. Astrophys., 348, 755-767 (1999)
	ISOGAL-DENIS detection of red giants with weak mass loss in the Galactic Bulge.
o	Table 2: <[OGA99] NNN> N=62 among (Nos 14-799) = <ISOGAL-P JHHMMSS.s+DDMMSS> N=62 = <DENIS-P JHHMMSS.s+DDMMSS> N=61.
Ref:	=2000JApA...21...77O
by	OJHA D.K. , OMONT A., GANESH S., SIMON G., SCHULTHEIS M.
	J. Astrophys. Astron., 21, 77-90 (2000)
	Stellar sources in the ISOGAL inner Galactic Bulge field (l = 0°, b = -1°).
o	Table 2: <[OOG2000] NNN> N=27 among (Nos 29-568) = <ISOGAL-P JHHMMSS.s+DDMMSS> N=27 = <DENIS-P JHHMMSS.s+DDMMSS> N=27.
Ref:	=2001ApJ...552..289A
by	ALARD C. , BLOMMAERT J.A.D.L., CESARSKY C., EPCHTEIN N., FELLI M., FOUQUE P., GANESH S., GENZEL R., GILMORE G., GLASS I.S., HABING H., OMONT A., PERAULT M., PRICE S., ROBIN A., SCHULTHEIS M., SIMON G., VAN LOON J.T., ALCOCK C., ALLSMAN R.A., ALVES D.R., AXELROD T.S., BECKER A.C., BENNETT D.P., COOK K.H., DRAKE A.J., FREEMAN K.C., GEHA M., GRIEST K., LEHNER M.J., MARSHALL S.L., MINNITI D., NELSON C., PETERSON B.A., POPOWSKI P., PRATT M.R., QUINN P.J., SUTHERLAND W., TOMANEY A.B., VANDEHEI T., WELCH D.L.
	Astrophys. J., 552, 289-308 (2001)
	Mass-losing semiregular variable stars in Baade's windows.
o	Table 1: <ISOGAL-P JHHMMSS.s+DDMMSS> N=332 = <[GGA99] NGC 6522 NNN> N=109 new, or = [GGA99] Sgr I NNN> N=152 new.
Ref:	=2002A&A...392..971F
by	FELLI M. , TESTI L., SCHULLER F., OMONT A.
	Astron. Astrophys., 392, 971-990 (2002)
	Young massive stars in the ISOGAL survey. II. The catalogue of bright YSO candidates.
o	Table 3: <ISOGAL-P JHHMMSS.s+DDMMSS> N=715.
Ref:	=2003A&A...403..955S
by	SCHULLER F. , GANESH S., MESSINEO M., MONETI A., BLOMMAERT J.A.D.L., ALARD C., ARACIL B., MIVILLE-DESCHENES M.-A., OMONT A., SCHULTHEIS M., SIMON G., SOIVE A., TESTI L.
	Astron. Astrophys., 403, 955-974 (2003)
	Explanatory supplement of the ISOGAL-DENIS. Point Source Catalogue.
o	<ISOGAL-P JHHMMSS.s+DDMMSS> N=106150.
=E=	Catalogue in electronic form as J/ApJ/552/289
=E=	Catalogue in electronic form as J/A+A/392/971
=E=	Catalogue in electronic form as II/243
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ISOHDF
ISOHDF	(Infrared Source Obs., Hubble Deep Field)
Write:	<<ISOHDF JHHMMSS.s+DDMMSS>>
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	ISO CAM observations of the HDF. See also [GOS97], [ACE99], [DPC99]
in source:	NAME HDFN
Ref:	=1997MNRAS.289..465G
by	GOLDSCHMIDT P. , OLIVER S.J., SERJEANT S.B.G., BAKER A., EATON N., EFSTATHIOU A., GRUPPIONI C., MANN R.G., MOBASHER B., ROWAN-ROBINSON M., SUMNER T.J., DANESE L., ELBAZ D., FRANCESCHINI A., EGAMI E., KONTIZAS M., LAWRENCE A., McMAHON R., NORGAARD-NIELSEN H.U., PEREZ-FOURNON I., GONZALEZ-SERRANO J.I.
	Mon. Not. R. Astron. Soc., 289, 465-470 (1997)
	Observations of the Hubble Deep Field with the Infrared Space Observatory - II. Source detection and photometry.
o	Tables 2, 3, 5, 6: <[GOS97] JHHMMSS.s+DDMMSS> = <ISOHDF JHHMMSS.s+DDMMSS> N=49.
Ref:	=1999A&A...342..313A
by	AUSSEL H. , CESARSKY C.J., ELBAZ D., STARCK J.L.
	Astron. Astrophys., 342, 313-336 (1999)
	ISOCAM observations of the Hubble Deep Field reduced with the PRETI method.
o	Table 6, HDF_{PS3}40 misprint for PM3_40 (in SIMBAD : [ACE99] HDF PM3.40 )
o	Table 3: <[ACE99] HDF PMN.NN> N=49, = <ISOHDF JHHMMSS.s+DDMMSS> N=49. Table 4: <[ACE99] HDF PSN.NNa> N=51 = <ISOHDF JHHMMSS.s+DDMMSS> N=51.
Ref:	=1999A&A...342..363D
by	DESERT F.-X. , PUGET J.-L., CLEMENTS D.L., PERAULT M., ABERGEL A., BERNARD J.-P., CESARSKY C.J.
	Astron. Astrophys., 342, 363-377 (1999)
	A classical approach to faint extragalactic source extraction from ISOCAM deep surveys. Application to the Hubble Deep Field.
o	Tables 1 to 5: <[DPC99] HDF-N-LWN-NN> = <ISOHDF JHHMMSS.s+DDMMSS>, N=4+2+18+15+23. Table 6: <[DPC99] HDF-ALL-LW3-NN> = <ISOHDF JHHMMSS.s+DDMMSS> N=41.
=E=	Catalogue in electronic form as J/A+A/342/313
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ISOHDFS
ISOHDFS	(Infrared Source Obs., Hubble Deep Field South)
Write:	<<ISOHDFS NN>>
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	ISOCAM detected sources.
in source:	NAME HDFS
Ref:	=2000ApJ...537L..85R
by	RIGOPOULOU D. , FRANCESCHINI A., AUSSEL H., GENZEL R., VAN DER WERF P., CESARSKY C.J., DENNEFELD M., OLIVER S., ROWAN-ROBINSON M., MANN R.G., PEREZ-FOURNON I., ROCCA-VOLMERANGE B.
	Astrophys. J., 537, 85-89 (2000)
	Very large Telescope-ISAAC near-infrared spectroscopy of ISO-selected Hubble Deep Field South galaxies.
o	Table 1: <ISOHDFS NN> N=12 among N=63.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ISOHDFS
ISOHDFS	(Infrared Source Obs., Hubble Deep Field South)
*****	Avoid the usage of ISOHDFS, prefer [OMC2002]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: ISOSS
ISOSS	(ISO Serendipity Survey)
Write:	<<ISOSS JHHMMm+DDMMa>>
N:	2000
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	The ISOPHOT Serendipity Survey utilized the otherwise unused slew time between ISO's pointed observations with strip scanning measurements at 170um. More than 12000 slew measurements exceeding 150000 degrees slew length and totaling nearly 550 hours of observing time were collected with ISOPHOT's 2x2 pixel C200 array, leading to an incomplete sky survey with a coverage of about 15%. Sources detected on the slews comprise mostly unresolved galaxies and compact galactic knots, which will be collected in the ISOSS source catalogue. 2000A&A...359..865S: 1st ref. with ISOSS objects. See also [SLK2000]. http://cdsweb.u-strasbg.fr/cgi-bin/Dic?ISOSS
Ref:	=2000A&A...359..865S
by	STICKEL M. , LEMKE D., KLAAS U., BEICHMAN C.A., ROWAN-ROBINSON M., EFSTATHIOU A., BOGUN S., KESSLER M.F., RICHTER G.
	Astron. Astrophys., 359, 865-875 (2000)
	The ISOPHOT 170µm serendipity survey. I. Compact sources with galaxy associations.
o	Table 4, col(1): <[SLK2000] NNN> (Nos 1-115) = Table 4, col(2): <ISOSS JHHMMm+DDMM> N=115.
=E=	Catalogue in electronic form as J/A+A/359/865
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: ISOY
ISOY	(Initial Spitzer Orion YSO)
Write:	<<ISOY JHHMMSS.ss+DDMMSS.s>>
N:	2067
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	N=2067 YSOs as part of the Spitzer GO6 Exploration Science program YSOVAR (Young Stellar Object Variability). See the program website: http://ysovar.ipac.caltech.edu/
in source:	NAME ONC
Ref:	=2011ApJ...733...50M
by	MORALES-CALDERON M. , STAUFFER J.R., HILLENBRAND L.A., GUTERMUTH R., SONG I., REBULL L.M., PLAVCHAN P., CARPENTER J.M., WHITNEY B.A., COVEY K., ALVES DE OLIVEIRA C., WINSTON E., McCAUGHREAN M.J., BOUVIER J., GUIEU S., VRBA F.J., HOLTZMAN J., MARCHIS F., HORA J.L., WASSERMAN L.H., TEREBEY S., MEGEATH T., GUINAN E., FORBRICH J., HUELAMO N., RIVIERE-MARICHALAR P., BARRADO D., STAPELFELDT K., HERNANDEZ J., ALLEN L.E., ARDILA D.R., BAYO A., FAVATA F., JAMES D., WERNER M., WOOD K.
	Astrophys. J., 733, 50 (2011)
	YSOVAR: the first sensitive, wide-area, mid-infrared photometric monitoring of the Orion Nebula Cluster.
o	Table 2: <ISOY JHHMMSS.ss+DDMMSS.s> N=2067.
=E=	Catalogue in electronic form as J/ApJ/733/50
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ISQ96]
[ISQ96]	(Infante+Slezak+Quintana, 1996)
Write:	<<[ISQ96] FFFA NN>> <<[ISQ96] FFFAN NN>>
N:	236
Object:	* (SIMBAD class: Star)
Note:	Tables 1-15: N=236 stars In the format 'FFF' stands for ESO fields 382, 383, 443, and 444, the letter 'A' stands for spots: spots C, F, G, K, L in ESO field 382. spots G, K, L in ESO field 383. spots M in ESO field 443: two tables of N=13 stars in the same spot, so we use a format '443M1 NN' (table 9) and '443M2 NN'(table 10). spots D, E, G, K, L in ESO field 444
Ref:	=1996A&AS..120..357I
by	INFANTE L. , SLEZAK E., QUINTANA H.
	Astron. Astrophys., Suppl. Ser., 120, 357-359 (1996)
	CCD sequences in the Shapley supercluster of galaxies. I. The LCO-Toronto telescope data.
o	PG 0918+29 misprint for PG 0918+029?
o	Tables 1-15: <[ISQ96] FFFA NN>, <[ISQ96] FFFAN NN> N=236
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ISS
ISS	(Intermediate Source Survey)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ISS
ISS	(Intermediate Source Survey)
Write:	<<ISS NN>>
N:	35
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Ref:	=1984Sci...225...23F
by	FOMALONT E.B. , KELLERMANN K.I., WALL J.V., WEISTROP D.
	Science, 225, 23-28 (1984)
	A deep 6-centimeter radio source survey.
o	Table 3: <[FKW84] DSS NN> (Nos 1-16). Table 4: <[FKW84] ISS NN> (Nos 1-35) = <ISS NN> (Nos 1-35).
Origin	of the Acronym: L (1993AJ....105...30M)
Details on Acronym: [ISS2013]
[ISS2013]	(Ivison+Swinbank+Smail+, 2013)
Write:	<<[ISS2013] A>> <<[ISS2013] galaxy>> <<[ISS2013] HATLAS J084933-A>> (not recognised by Simbad, but found in literature)
N:	5+1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	NRAO JVLA (CO J=1-0 and 5GHz), CARMA (CO J=3-2), IRAM PdBI (CO J=4-3), SMA (870µm), CSO SHARC-2 (350µm), Hershel SPIRE and PACS, Spitzer IRAC, HST WFC3, and Keck II DEIMOS observations of N=5 galaxies. N=1 lenticular galaxy that lies along the line of sight to component T.
in source:	H-ATLAS J084933.4+021443
Ref:	=2013ApJ...772..137I
by	IVISON R.J. , SWINBANK A.M., SMAIL I., HARRIS A.I., BUSSMANN R.S., COORAY A., COX P., FU H., KOVACS A., KRIPS M., NARAYANAN D., NEGRELLO M., NERI R., PENARRUBIA J., RICHARD J., RIECHERS D.A., ROWLANDS K., STAGUHN J.G., TARGETT T.A., AMBER S., BAKER A.J., BOURNE N., BERTOLDI F., BREMER M., CALANOG J.A., CLEMENTS D.L., DANNERBAUER H., DARIUSH A., DE ZOTTI G., DUNNE L., EALES S.A., FARRAH D., FLEUREN S., FRANCESCHINI A., GEACH J.E., GEORGE R.D., HELLY J.C., HOPWOOD R., IBAR E., JARVIS M.J., KNEIB J.-P., MADDOX S., OMONT A., SCOTT D., SERJEANT S., SMITH M.W.L., THOMPSON M.A., VALIANTE E., VALTCHANOV I., VIEIRA J., VAN DER WERF P.
	Astrophys. J., 772, 137 (2013)
	Herschel-ATLAS: a binary HyLIRG pinpointing a cluster of starbursting protoellipticals.
o	Fig. 1, Table 2: <[ISS2013] A> (Nos C, M, T, W). Fig. 1, Paragr. 3.2: <[ISS2013] galaxy> N=1.
Ref:	=2019MNRAS.489..427I
by	IVISON R.J. , PAGE M.J., CIRASUOLO M., HARRISON C.M., MAINIERI V., ARUMUGAM V., DUDZEVICIUTE U.
	Mon. Not. R. Astron. Soc., 489, 427-436 (2019)
	Hyperluminous starburst gives up its secrets.
o	Fig. 4, Table 1: <[ISS2013] A> (No. E) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ISW2008]
[ISW2008]	(Ikeda+Sugitani+Watanabe+, 2008)
Write:	<<[ISW2008] {E\|I\|R}NN>>
N:	10+6+3
Object:	Em* + (Near IR) (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	Wide Field Grism Spectrograph 2 of the University of Hawaii 2.2m telescope observations of the bright-rimmed cometary (BRC) globule SFO 37 in IC 1396. See also [OSP2002].
in source:	IC 1396:SFO 37 = SFO 37
Ref:	=2008AJ....135.2323I
by	IKEDA H. , SUGITANI K., WATANABE M., FUKUDA N., TAMURA M., NAKAJIMA Y., PICKLES A.J., NAGASHIMA C., NAGAYAMA T., NAKAYA H., NAKANO M., NAGATA T.
	Astron. J., 135, 2323-2335 (2008)
	Sequential star formation in a cometary globule (BRC37) of IC1396.
o	Table 1, Fig.1: <[ISW2008] ENN> (Nos E1-E10). Table 2, Fig.2: <[ISW2008] IN> (Nos I1-I6), <[ISW2008] RN> (Nos R1-R3). Table 4: <[OSP2002] BRC NN NN>, <[OSP2002] BRC NNWW NN>, <[OSP2002] Cep B NN>, <[OSP2002] LW Cas NN>, <[OSP2002] OriI-2N N>, N=31 added, <[OSP2002] BRC 13 NNa> (Nos 6a-6b) added.
=E=	Catalogue in electronic form as <J/AJ/135/2323/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ISW2010]
[ISW2010]	(Ishwara-Chandra+Sirothia+Wadadekar+, 2010)
Write:	<<[ISW2010] GMRT JHHMMSS+DDMMSS>>
N:	765
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	GMRT 150MHz observations of the LBDS-Lynx region.
in source:	NAME Lynx Region
Ref:	=2010MNRAS.405..436I
by	ISHWARA-CHANDRA C.H. , SIROTHIA S.K., WADADEKAR Y., PAL S., WINDHORST R.
	Mon. Not. R. Astron. Soc., 405, 436-446 (2010)
	Deep GMRT 150-MHz observations of the LBDS-Lynx region: ultrasteep spectrum radio sources.
o	Table 3: <[ISW2010] GMRT JHHMMSS+DDMMSS> N=765.
=E=	Catalogue in electronic form as <J/MNRAS/405/436/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IsWe
IsWe	(Ishida+Weinberger)= (IW)
Write:	<<PN IsWe N>>
N:	2
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	Maps
Ref:	=1987A&A...178..227I
by	ISHIDA K. , WEINBERGER R.
	Astron. Astrophys., 178, 227-236 (1987)
	Two senile nearby planetary nebulae and the local planetary nebulae population.
o	Table 3: <PN IsWe N> (Nos 1-2)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [IT2009]
[IT2009]	(Izotov+Thuan, 2009)
Write:	<<[IT2009] SN>>
N:	1
Object:	SN (SIMBAD class: Supernova = SuperNova)
Stat:	is completely incorporated in Simbad
Note:	APO 3.5m telescope optical observations of N=1 supernova in the dwarf galaxy SDSS J132053.66+215510.2.
in source:	SDSS J132053.0+215510.0
Ref:	=2009ApJ...707.1560I
by	IZOTOV Yu.I. , THUAN T.X.
	Astrophys. J., 707, 1560-1565 (2009)
	A type IIn supernova with coronal lines in the low-metallicity compact dwarf galaxy J1320+2155.
o	<[IT2009] SN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: ITG
ITG	(Itoh+Tamura+Gatley)
Write:	<<ITG NNA>> <<ITG NN-FN>>
N:	50+7+8
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	ITG survey (description in 1996ApJ...465L.129I). (Nos 1-50): Search for YSO candidates. Format 'NNA' for YSO candidate companions. Format 'NN-FN' for background sources.
in source:	TMC-COMPLEX
Ref:	=1998Sci...282.1095T
by	TAMURA M. , ITOH Y., OASA Y., NAKAJIMA T.
	Science, 282, 1095-1097 (1998)
	Isolated and companion young brown dwarfs in the Taurus and Chamaleon molecular clouds.
o	Complete list of ITG objects in 1999AJ....117.1471I, complete list of OTS objects in 1999ApJ...526..336O.
o	Table 1: <ITG NNA> N=7 among (Nos 9B and 45B), <OTS NN> N=6 among (Nos 7-48).
Ref:	=1999AJ....117.1471I
by	ITOH Y. , TAMURA M., NAKAJIMA T.
	Astron. J., 117, 1471-1484 (1999)
	A near-infrared search for companions around very low luminosity young stellar objects in Taurus.
o	T.6: cross-id 'Kim' not in SIMBAD.
o	Table 6: <ITG NN> (Nos 1-50). Table 3: <ITG NN-FN> N=8.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [ITH2008]
[ITH2008]	(Itoh+Tamura+Hayashi+, 2008)
Write:	<<[ITH2008] AA Tau-ccN>> <<[ITH2008] HBC NNN-ccN>> <<[ITH2008] HD NNNNNNA-ccN>> <<[ITH2008] HDE NNNNNN-ccN>> <<[ITH2008] RX JHHMM.m+DDMM-ccN>> <<[ITH2008] VNNN Tau-ccN>> <<[ITH2008] LkCa NN-ccN>>
N:	54
Object:	YSO companion (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Subaru NIR coronograph camera observations of N=32 YSOs to search for faint companions.
Ref:	=2008PASJ...60..209I
by	ITOH Y. , TAMURA M., HAYASHI M., OASA Y., HAYASHI S.S., FUKAGAWA M., KUDO T., MAYAMA S., ISHII M., PYO T.-S., YAMASHITA T., MORINO J.
	PASJ, 60, 209-218 (2008)
	Near-infrared spectroscopy of faint companions around young stellar objects associated with the Taurus molecular cloud.
o	Fig.1, Table 1: <[ITH2008] AA Tau-ccN>, <[ITH2008] HBC NNN-ccN>, <[ITH2008] HD NNNNNNA-ccN>, <[ITH2008] HDE NNNNNN-ccN>, <[ITH2008] RX JHHMM.m+DDMM-ccN>, <[ITH2008] VNNN Tau-ccN>, <[ITH2008] LkCa NN-ccN>, N=54.
=E=	Catalogue in electronic form as J/PASJ/60/209
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ITK2017]
[ITK2017]	(Itoh+Tanaka+Kawabata+, 2017)
Write:	<<[ITK2017] FSN>>
N:	7
Object:	* (SIMBAD class: Star)
Note:	Kanata Telescope spesctroscopic observations of N=7 field stars around V404 Cygni.
Ref:	=2017PASJ...69...25I
by	ITOH R. , TANAKA Y.T., KAWABATA K.S., UEMURA M., WATANABE M., KUKAZAWA Y., KANDA Y., AKITAYA H., MORITANI Y., NAKAOKA T., KAWABATA M., SHIKI K., YOSHIDA M., OASA Y., TAKAHASHI J.
	PASJ, 69, 25 (2017)
	A measurement of interstellar polarization and an estimation of Galactic extinction for the direction of the X-ray black hole binary V404 Cygni.
o	Tables 1,3: <[ITK2017] FSN> (Nos FS1-FS7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ITL2019]
[ITL2019]	(Issac+Tej+Liu+, 2019)
Write:	<<[ITL2019] RN>> <<[ITL2019] SMAN>> <<[ITL2019] CNN>>
N:	2+3+12
Object:	(Rad) + mm core + Clump (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	GMRT (610 and 1390MHz), SMA (1.1mm), and UKIRT (NIR) observations of N=2 radio components, N=3 millimeter cores, and N=12 clumps in the field of EGO G012.42+0.50.
Ref:	=2019MNRAS.485.1775I
by	ISSAC N. , TEJ A., LIU T., VARRICATT W., VIG S., ISHWARA CHANDRA C.H., SCHULTHEIS M.
	Mon. Not. R. Astron. Soc., 485, 1775-1799 (2019)
	Initial phases of high-mass star formation: a multiwavelength study towards the extended green object G12.42+0.50.
o	Fig. 2, Table 4: <[ITL2019] RN> (Nos R1-R2). Fig. 7, Table 6: <[ITL2019] SMAN> (Nos SMA1-SMA3). Fig. 9, Table 8: <[ITL2019] CNN> (Nos C1-C12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ITS2007]
[ITS2007]	(Izotov+Thuan+Stasinska, 2007)
Write:	<<[ITS2007] NNNNN-NNNN-NNN>>
N:	271
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	HII regions selected from the SDSS DR5. In the format the first NNNNN stands for the middle Julian date (MJD) of the observation, the second NNNN for the plate number, and the last NNN for the fiber number.
Ref:	=2007ApJ...662...15I
by	IZOTOV Y.I. , THUAN T.X., STASINSKA G.
	Astrophys. J., 662, 15-38 (2007)
	The primordial abundance of ^{4}He: a self-consistent empirical analysis of systematic effects in a large sample of low-metallicity H II regions.
o	Table 1: <[ITS2007] NNNNN-NNNN-NNN> N=271.
=E=	Catalogue in electronic form as J/ApJ/662/15
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [ITS2017]
[ITS2017]	(Izzo+Thone+Schulze+, 2017)
Write:	<<[ITS2017] HII-N>>
N:	8
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	VLT MUSE observations of N=8 HII regions in the host galaxy of GRB 100316D.
in source:	Anon J071031-5615
Ref:	=2017MNRAS.472.4480I
by	IZZO L. , THONE C.C., SCHULZE S., MEHNER A., FLORES H., CANO Z., DE UGARTE POSTIGO A., KANN D.A., AMORIN R., ANDERSON J.P., BAUER F.E., BENSCH K., CHRISTENSEN L., COVINO S., DELLA VALLE M., FYNBO J.P.U., JAKOBSSON P., KLOSE S., KUNCARAYAKTI H., LELOUDAS G., MILVANG-JENSEN B., MOLLER P., PUECH M., ROSSI A., SANCHEZ-RAMIREZ R., VERGANI S.D.
	Mon. Not. R. Astron. Soc., 472, 4480-4496 (2017)
	The MUSE view of the host galaxy of GRB 100316D.
o	Table 1: <[ITS2017] HII-N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IUM2019]
[IUM2019]	(Inno+Urbaneja+Matsunaga+, 2019)
Write:	<<[IUM2019] ID-N>>
N:	5
Object:	Cepheid (SIMBAD class: Cepheid = Cepheid Variable)
Stat:	is completely incorporated in Simbad
Note:	IRSF 1.4m telescope SIRIUS near-IR observations of N=5 cepheids in the Galactic disk. In the format, 'ID' stands for 'inner disk'.
Ref:	=2019MNRAS.482...83I
by	INNO L. , URBANEJA M.A., MATSUNAGA N., BONO G., NONINO M., DEBATTISTA V.P., SORMANI M.C., BERGEMANN M., DA SILVA R., LEMASLE B., ROMANIELLO M., RIX H.-W.
	Mon. Not. R. Astron. Soc., 482, 83-97 (2019)
	First metallicity determination from near-infrared spectra for five obscured Cepheids discovered in the inner disc.
o	Table 1, Fig. 1: <[IUM2019] ID-N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IUY2001]
[IUY2001]	(Ishisaki+Ueda+Yamashita+, 2001)
Write:	<<[IUY2001] NN>>
N:	50
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ASCA SIS observations of the Lockman Hole. ROSAT observations are compared with ASCA ones.
in source:	NAME Lockman Hole
Ref:	=2001PASJ...53..445I
by	ISHISAKI Y. , UEDA Y., YAMASHITA A., OHASHI T., LEHMANN I., HASINGER G.
	Publ. Astron. Soc. Jap., 53, 445-457 (2001)
	ASCA Deep survey in the Lockman Hole Field.
o	Table 2: <[IUY2001] NN> N=50 among (Nos 1-59).
=E=	Catalogue in electronic form as J/PASJ/53/445
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IV2001]
[IV2001]	(Iglesias-Paramo+Vilchez, 2001)= (TD) (Not yet in Simbad)
Write:	<<[IV2001] TD NNa>>
N:	36
Object:	Star-forming object (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=36 tidal dwarf (TD) galaxies candidates in HCG NNa parent galaxies. Maps in Figs 1-5.
in source:	HCG 31
in source:	HCG 44
in source:	HCG 92 = Stephan's Quintet
in source:	HCG 93
in source:	HCG 95
Ref:	=2001ApJ...550..204I
by	IGLESIAS-PARAMO J. , VILCHEZ J.M.
	Astrophys. J., 550, 204-211 (2001)
	Star-forming objects in the tidal tails of compact groups.
o	Table 1: <[IV2001] TD 31a> (Nos 31a-31i), <[IV2001] TD 44a> (Nos 44a-44h>, <[IV2001] TD 92a> (Nos 92a-92g>, <[IV2001] TD 93a> (Nos 93a-93h>, <[IV2001] TD 95a> (Nos 95a-95d).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IV74]
[IV74]	(Israel+Van Der Kruit, 1974)= (IK)
Write:	<<[IV74] NN>> <<[IV74] A>>
N:	67+12
Object:	HII (Rad) + (Rad) (SIMBAD class: Radio = Radio Source)
Note:	Identif. charts. Table 2(a): (Nos 1-67). Table 2(b): (Nos A-L).
in source:	M 33 = NGC 598
Ref:	=1974A&A....32..363I
by	ISRAEL F.P. , VAN DER KRUIT P.C.
	Astron. Astrophys., 32, 363-374 (1974)
	Radio observations of HII regions in external galaxies.
o	Table 2(a): <[IV74] NN>, N=67. Table 2(b): <[IV74] A>, N=12
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IV98]
[IV98]	(Iglesias-Paramo+Vilchez, 1998) (Not yet in Simbad)
Write:	<<[IV98] AN>> <<[IV98] Northern Tail>> <<[IV98] Bridge>>
N:	2+1+1+5
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Observations of HCG 95. The 2 galaxies C1 and C2 are forming a triplet with HCG 95A. Observations of a 'Northern Tail' and a 'Bridge', with N=5 Knots (Nos K1-K5) in the Northern Tail.
in source:	HCG 95
Ref:	=1998AJ....115.1791I
by	IGLESIAS-PARAMO J. , VILCHEZ J.M.
	Astron. J., 115, 1791-1800 (1998)
	Detailed photometric study of the merging group of galaxies HCG 95.
o	Table 3, Fig.1: <[IV98] CN> (Nos C1-C2), <[IV98] Northern Tail> N=1, <[IV98] Bridge> N=1, <[IV98] KN> (Nos K1-K5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Ivanov
Ivanov	(Ivanov)
*****	Avoid the usage of Ivanov, prefer [IBP2002]
Origin	of the Acronym: L (2010A&A...516A...3K)
Details on Acronym: IVC
IVC	(Intermediate-Velocity Cloud)
Write:	<<IVC LLL.l+BB.b-VV>>
Object:	IVC (SIMBAD class: Cloud)
Note:	Systematic designation. The term IVC is traditionally reserved for clouds having velocity between 35 and 80 km/s. See HVC, LVC. See also [H75b], Giovanelli
Details on Acronym: [IVE99]
[IVE99]	(Immler+Vogler+Ehle+, 1999)
Write:	<<[IVE99] HNN>> <<[IVE99] DN>>
N:	37+4
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations of M 83: N=37 sources (Nos H1-H37). N=4 variable sources, letter D stands for Difference, referring to the fact that X-ray emission deviates significantly during the period of observation. See also ROSAT PSPC sources, [EPB98].
in source:	M 83 = NGC 5236
Ref:	=1999A&A...352..415I
by	IMMLER S. , VOGLER A., EHLE M., PIETSCH W.
	Astron. Astrophys., 352, 415-430 (1999)
	ROSAT high-resolution X-ray observations of M 83: detection of supernova remnant and black hole candidates.
o	Table 3: <[IVE99] HNN> (Nos H1-H37). Table 4: <[IVE99] DN> (Nos D1-D4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IVM2003]
[IVM2003]	(Infante+Varela+Moles+, 2003)
Write:	<<[IVM2003] cnd FF>> <<[IVM2003] cnd FF-N>>
N:	12
Object:	Poss. QSO (SIMBAD class: QSO_Candidate = Quasar Candidate)
Note:	Search for QSO candidates at a redshift similar to that of the target QSO. In the format 'FF' designates the field where the candidate is found, when there are several candidates in the same field the format is FF-1, FF-2...
Ref:	=2003ApJ...588...90I
by	INFANTE L. , VARELA J., MOLES M., HERTLING G., GARCIA A., MENANTEAU F.
	Astrophys. J., 588, 90-98 (2003)
	Quasars clustering at z~3 on scales ≲10 h^{-1} mpc.
o	Table 6: <[IVM2003] cnd FF>, <[IVM2003] cnd FF-N>, N=12.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IVR2011]
[IVR2011]	(Intema+van Weeren+Roettgering+, 2011)
Write:	<<[IVR2011] JHHMMSS+DDMMSS>>
N:	598
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	GMRT 153MHz observations of N=598 sources in the NOAO Bootes Field. See also [WIR2013].
in source:	NAME Bootes Field
Ref:	=2011A&A...535A..38I
by	INTEMA H.T. , VAN WEEREN R.J., ROETTGERING H.J.A., LAL D.V.
	Astron. Astrophys., 535A, 38-38 (2011)
	Deep low-frequency radio observations of the NOAO Bootes field. I. Data reduction and catalog construction.
o	Table 3: <[IVR2011] JHHMMSS+DDMMSS> N=598.
=E=	Catalogue in electronic form as <J/A+A/535/A38/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IVS
IVS	(International VLBI Service)
Write:	<<IVS BHHMM+DDd>> <<IVS BHHMM+DDA>>
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Extragalactic radio-sources in the northern sky, used as VLBA calibrators. IVS sources are also IERS sources. See also VCS1 to VCS6 J2000 designation for IVS sources. Since about 2010, the Radio Fundamental Catalog (http://astrogeo.org/rfc/) also maintains a list of IVS sources, that are not only calibrators.
Ref:	=2002ApJS..141...13B
by	BEASLEY A.J. , GORDON D., PECK A.B., PETROV L., MacMILLAN D.S., FOMALONT E.B., MA C.
	Astrophys. J., Suppl. Ser., 141, 13-21 (2002)
	The VLBA calibrator Survey–VCS1.
o	Tables 2, 4: <VCS1 JHHMM+DDMM> N=1332+72 = <IVS BHHMM+DDd> N=1332+72.
Ref:	=2003AJ....126.2562F
by	FOMALONT E.B. , PETROV L., MacMILLAN D.S., GORDON D., MA C.
	Astron. J., 126, 2562-2566 (2003)
	The second VLBA calibrator survey: VCS2.
o	Table 3, col(1): <VCS2 JHHMM+DDMM> N=276 = Table 3, col(2): <IVS BHHMM+DDd> N=276.
Ref:	=2005AJ....129.1163P
by	PETROV L. , KOVALEV Y.Y., FOMALONT E., GORDON D.
	Astron. J., 129, 1163-1170 (2005)
	The third VLBA calibrator survey: VCS3.
o	Table 2, col(2): <IVS BHHMM+DDd> N=360 = Table 2, col(3): <VCS3 JHHMM+DDMM> N=360.
Ref:	=2006AJ....131.1872P
by	PETROV L. , KOVALEV Y.Y., FOMALONT E.B., GORDON D.
	Astron. J., 131, 1872-1879 (2006)
	The fourth VLBA calibrator survey: VCS4.
o	Table 2, col(2): <IVS BHHMM+DDd> N=258 = Table 2, col(3): <VCS3 JHHMM+DDMM> N=258.
Ref:	=2007AJ....133.1236K
by	KOVALEV Y.Y. , PETROV L., FOMALONT E.B., GORDON D.
	Astron. J., 133, 1236-1242 (2007)
	The fifth VLBA calibrator survey: VCS5.
o	Table 2, col(2): <IVS BHHMM+DDd> N=569 = Table 2, col(3): <VCS5 JHHMM+DDMM> N=569.
o	Objets from table 2 are designated in Simbad with their NVSS name.
Ref:	=2008AJ....136..580P
by	PETROV L. , KOVALEV Y.Y., FOMALONT E.B., GORDON D.
	Astron. J., 136, 580-585 (2008)
	The sixth VLBA calibrator survey: VCS6.
o	Table 4, col(2): <IVS BHHMM+DDd> N=264 = Table 4, col(3): <VCS6 JHHMM+DDMM> N=264.
Ref:	=2011AJ....142...35P
by	PETROV L. , KOVALEV Y.Y., FOMALONT E.B., GORDON D.
	Astron. J., 142, 35 (2011)
	The Very Long Baseline Array Galactic Plane Survey–VGaPS.
o	Table 9: <IVS BHHMM+DDd> N=327.
Ref:	=2011AJ....142...89P
by	PETROV L. , TAYLOR G.B.
	Astron. J., 142, 89 (2011)
	Precise absolute astrometry from the VLBA imaging and polarimetry survey at 5 GHz.
o	Table 2: <IVS BHHMM+DDd> N=857.
Ref:	=2011AJ....142..105P
by	PETROV L.
	Astron. J., 142, 105 (2011)
	The catalog of positions of optically bright extragalactic radio sources OBRS-1.
o	Table 2: <IVS BHHMM+DDd> N=105.
Ref:	=2012AJ....143...35P
by	PETROV L. , HONMA M., SHIBATA S.M.
	Astron. J., 143, 35 (2012)
	The KCAL VERA 22 GHz calibrator survey.
o	Table 3: <IVS BHHMM+DDd> N=877.
Ref:	=2012AJ....144..150P
by	PETROV L. , LEE S.-S., KIM J., JUNG T., OH J., SOHN B.W., BYUN D.-Y., CHUNG M.-H., JE D.-H., WI S.-O., SONG M.-G., KANG J., HAN S.-T., LEE J.-W., KIM B.G., CHUNG H., KIM H.-G.
	Astron. J., 144, 150 (2012)
	Early science with the Korean VLBI Network: the QCAL-1 43 GHz Calibrator Survey.
o	Tables 3-4: <IVS BHHMM+DDd> N=637+33.
Ref:	=2012MNRAS.419.1097P
by	PETROV L.
	Mon. Not. R. Astron. Soc., 419, 1097-1106 (2012)
	The EVN galactic plane survey - EGaPS.
o	Tables 3-4: <IVS BHHMM+DDd> N=9+109.
Ref:	=2013AJ....146....5P
by	PETROV L.
	Astron. J., 146, 5 (2013)
	The catalog of positions of optically bright extragalactic radio sources OBRS-2.
o	Table 2: <IVS BHHMM+DDd> N=295.
=E=	Catalogue in electronic form as <J/ApJS/141/13/>
=E=	Catalogue in electronic form as <J/AJ/126/2562/>
=E=	Catalogue in electronic form as <J/AJ/129/1163/>
=E=	Catalogue in electronic form as <J/AJ/131/1872/>
=E=	Catalogue in electronic form as <J/AJ/133/1236/>
=E=	Catalogue in electronic form as <J/AJ/136/580/>
=E=	Catalogue in electronic form as <J/MNRAS/419/1097/>
=E=	Catalogue in electronic form as <J/AJ/142/35/>
=E=	Catalogue in electronic form as <J/AJ/142/89/>
=E=	Catalogue in electronic form as <J/AJ/143/35/>
=E=	Catalogue in electronic form as <J/AJ/142/105/>
=E=	Catalogue in electronic form as <J/AJ/144/150/>
=E=	Catalogue in electronic form as <J/AJ/146/5/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: IW
IW	(Ishida+Weinberger)
*****	Avoid the usage of IW, prefer IsWe
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [IW2001]
[IW2001]	(Immler+Wang, 2001)
Write:	<<[IW2001] HNN>> <<[IW2001] PNN>>
N:	46+69
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI and PSPC observations of M 81. HRI sources format 'HNN', PSPC sources format 'PNN'.
in source:	M 81 = NGC 3031
Ref:	=2001ApJ...554..202I
by	IMMLER S. , WANG Q.D.
	Astrophys. J., 554, 202-215 (2001)
	ROSAT X-ray observations of the spiral galaxy M81.
o	Table 3: <[IW2001] HNN> (Nos H1-H46). Table 4: <[IW2001] PNN> (Nos P1-P69).
=E=	Catalogue in electronic form as J/ApJ/554/202
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IW83]
[IW83]	(Israel+Wootten, 1983) (Not yet in Simbad)
Write:	<<[IW83] Cyg MC1 W>> <<[IW83] 1-NN>> <<[IW83] 3-N>>
N:	2+13+7
Object:	CO Cloud (SIMBAD class: Cloud)
Note:	N=2 complexes of CO clouds, 'Cyg MC1 West' west of Onsala 1, and Cyg MC1 East' east of Onsala 1. Tables 1 and 3 list CO clouds with 8' and 2'.3 resolution respectively.
Ref:	=1983ApJ...266..580I
by	ISRAEL F.P. , WOOTTEN H.A.
	Astrophys. J., 266, 580-595 (1983)
	The molecular cloud complex associated with ON 1.
o	<[IW83] Cyg MC1 W> (Nos W, E). Table 1: <[IW83] 1-NN> (Nos 1-1 to 1-13). Table 3: <[IW83] 3-N> (Nos 3-1 to 3-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IWG97]
[IWG97]	(Ibata+Wyse+Gilmore+, 1997) (Not yet in Simbad)
Write:	<<[IWG97] HHMMSS.ss+DDMMSS.s>>
N:	229+270
Object:	* (SIMBAD class: Star)
in source:	NAME SDG = NAME Sgr Dwarf Galaxy
Ref:	=1997AJ....113..634I
by	IBATA R.A. , WYSE R.F.G., GILMORE G., IRWIN M.J., SUNTZEFF N.B.
	Astron. J., 113, 634-655 (1997)
	The kinematics orbit and survival of the Sagittarius dwarf spheroidal galaxy.
o	Table 2(a), 2(b): <[IWG97] HHMMSS.ss-DDMMSS> N=229+270
=E=	Catalogue in electronic form as J/AJ/113/634
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IWL2003]
[IWL2003]	(Immler+Wang+Leonard+, 2003)
Write:	<<[IWL2003] NN>>
N:	79
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of NGC 1637.
in source:	NGC 1637
Ref:	=2003ApJ...595..727I
by	IMMLER S. , WANG Q.D., LEONARD D.C., SCHLEGEL E.M.
	Astrophys. J., 595, 727-742 (2003)
	A deep Chandra X-ray observation of NGC 1637.
o	Source 1 in M 82 = [WSG84] 1
o	Table 3: <[IWL2003] NN> (Nos 1-79).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IWO2002]
[IWO2002]	(Imai+Watanabe+Omodaka+, 2002) (Not yet in Simbad)
Write:	<<[IWO2002] W51N NNN>> <<[IWO2002] W51M NN>> <<[IWO2002] W51S NN>>
N:	123+48+10
Object:	H2O Maser (SIMBAD class: Maser)
in source:	W 51
Ref:	=2002PASJ...54..741I
by	IMAI H. , WATANABE T., OMODAKA T., NISHIO M., KAMEYA O., MIYAJI T., NAKAJIMA J.
	Publ. Astron. Soc. Jap., 54, 741-755 (2002)
	3-D kinematics of water masers in the W 51A region.
o	Table 2: <[IWO2002] W51N NNN> (Nos 1-123). Table 3: <[IWO2002] W51M NN> (Nos 1-48). Table 4: <[IWO2002] W51SNN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IWO86]
[IWO86]	(Ichikawa+Wakamatsu+Okamura, 1986)
Write:	<<[IWO86] NN>> <<[IWO86] SN>>
N:	69+7
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	N=69 elliptical G, and N=7 Spiral G (Nos S1-S7)
in source:	NAME Virgo Cluster
Ref:	=1986ApJS...60..475I
by	ICHIKAWA S.-I. , WAKAMATSU K.-I., OKAMURA S.
	Astrophys. J., Suppl. Ser., 60, 475-506 (1986)
	Surface photometry of dwarf elliptical galaxies in the Virgo cluster.
o	(Erratum) + erratum vol 62, 253
o	<[IWO86] NN> N=69, <[IWO86] SN> N=7
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IWZ2014]
[IWZ2014]	(Ishioka+Wang+Zhang+, 2014)= (TAOS)
Write:	<<TAOS TAOS FFF.NNNNN>>
N:	164+58
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	N=158 known and N=58 new variable stars from the Taiwan-American Occultation Survey project (TAOS). More information at: http://taos.asiaa.sinica.edu.tw/index.php
Ref:	=2014AJ....147...70I
by	ISHIOKA R. , WANG S.-Y., ZHANG Z.-W., LEHNER M.J., ALCOCK C., AXELROD T., BIANCO F.B., BYUN Y.-I., CHEN W.P., COOK K.H., KIM D.-W., KING S.-K., LEE T., MARSHALL S.L., PROTOPAPAS P., RICE J.A., SCHWAMB M.E., WANG J.-H., WEN C.-Y., NGEOW C.-C.
	Astron. J., 147, 70 (2014)
	The Taiwanese-American Occultation Survey project stellar variability. III. Detection of 58 new variable stars.
o	Tables 5-6: <[IWZ2014] TAOS FFF.NNNNN> N=164+58 added.
=E=	Catalogue in electronic form as J/AJ/147/70
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: IXO
IXO	(Intermediate-luminosity X-ray Object)
Write:	<<IXO NN>>
N:	87
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	N=87 ROSAT HRI Intermediate-luminosity X-ray extranuclear Objects.
Ref:	=2002ApJS..143...25C
by	COLBERT E.J.M. , PTAK A.F.
	Astrophys. J., Suppl. Ser., 143, 25-45 (2002)
	A catalog of candidate intermediate-luminosity X-ray objects.
o	Table 1: <IXO NN> (Nos 1-87).
=E=	Catalogue in electronic form as J/ApJS/143/25
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [IYE2006]
[IYE2006]	(Iono+Yun+Elvis+, 2006)
Write:	<<[IYE2006] BR 1202W>>
N:	2
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SMA observations of QSO BR 1202-0725 which is resolved into 2 submillimeter components.
in source:	BR B1202-0725
Ref:	=2006ApJ...645L..97I
by	IONO D. , YUN M.S., ELVIS M., PECK A.B., HO P.T.P., WILNER D.J., HUNTER T.R., MATSUSHITA S., MULLER S.
	Astrophys. J., 645, 97-100 (2006)
	A detection of [C II] line emission in the z = 4.7 QSO BR 1202-0725.
o	Fig.1, Table 2: <[IYE2006] BR 1202W> (Nos N, S).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IYS2008]
[IYS2008]	(Ito+Yamashita+Sako+, 2008)
Write:	<<[IYS2008] {J\|H\|K}NN>> <<[IYS2008] NSN>>
N:	15+17+10+9
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	Subaru AO IRCS observations in the J, H, and K bands. Search for YSO silhouette objects in M 17.
in source:	M 17 = NGC 6618
Ref:	=2008ApJ...672..398I
by	ITO M. , YAMASHITA T., SAKO S., TAKAMI H., HAYANO Y., TERADA H.
	Astrophys. J., 672, 398-409 (2008)
	Near-infrared silhouette object survey in M17.
o	Figs 3-6, Table 3: <[IYS2008] JNN> (Nos J1-J15), <[IYS2008] HNN> (Nos H1-H17), <[IYS2008] KNN> (Nos K1-K10), <[IYS2008] NSN> (Nos NS1-NS9).
=E=	Catalogue in electronic form as J/ApJ/672/398
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IZH2021]
[IZH2021]	(Indahl+Zeimann+Hill+, 2021) (Not yet in Simbad)
Write:	<<[IZH2021] O3ELGNNa>>
N:	18
Object:	Em. G (SIMBAD class: EmissionG = Emission-line galaxy)
Note:	HET LRS2 observations of N=18 low-metallicity galaxies, selected in early data from the Hobby–Eberly Telescope Dark Energy Experiment (HETDEX).
Ref:	=2021ApJ...916...11I
by	INDAHL B. , ZEIMANN G., HILL G.J., BOWMAN W.P., CIARDULLO R., DRORY N., GAWISER E., HOPP U., JANOWIECKI S., BOYLAN-KOLCHIN M., MENTUCH COOPER E., DAVIS D., FARROW D., FINKELSTEIN S., GRONWALL C., KELZ A., McQUINN K.B.W., SCHNEIDER D., TUTTLE S.E.
	Astrophys. J., 916, 11-11 (2021)
	HETDEX [O III] emitters. I. A spectroscopically selected low-redshift population of low-mass, low-metallicity galaxies.
o	Fig. 1, Tables 1-6: <[IZH2021] O3ELGNNa> (Nos O3ELG1-O3ELG3, O3ELG4a-O3ELG4b, O3ELG5-O3ELG11, O3ELG12a-O3ELG12b, O3ELG13-O3ELG16).
=E=	Catalogue in electronic form as <J/ApJ/916/11/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [IZL2015]
[IZL2015]	(Infante+Zheng+Laporte+, 2015)
Write:	<<[IZL2015] NNNN>>
Object:	Poss. G (SIMBAD class: Galaxy_Candidate = Galaxy Candidate)
Note:	N=22 galaxy candidates at z≥7 in the field of the strong-lensing cluster MCS J0416.0-2403 and the associated parallel field. Use of HST ACS and WFC3 data from the Hubble Frontier Fields (HFF) program. Use of Hubble and Spitzer photometry.
in source:	MCS J0416.1-2403
Ref:	=2015ApJ...815...18I
by	INFANTE L. , ZHENG W., LAPORTE N., TRONCOSO IRIBARREN P., MOLINO A., DIEGO J.M., BAUER F.E., ZITRIN A., MOUSTAKAS J., HUANG X., SHU X., BINA D., BRAMMER G.B., BROADHURST T., FORD H.C., GARCIA S., KIM S.
	Astrophys. J., 815, 18 (2015)
	Young galaxy candidates in the Hubble frontier fields. II. MACS J0416-2403.
o	Figs 1-2, Tables 2-6: <[IZL2015] NNNN> N=22 among (Nos 146-8958).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: J
J	(Jones ?)
*****	Avoid the usage of J, prefer [HJS91]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: J
J	(Jacoby)
*****	Avoid the usage of J, prefer [J79]
Origin	of the Acronym: L (1996ApJ...472..711G)
Details on Acronym: J
J	(Jacoby)
*****	Avoid the usage of J, prefer Jacoby
Origin	of the Acronym: L = Found in the literature
Details on Acronym: J
J	(Jorgensen+)
*****	Avoid the usage of J, prefer [JFK95]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: J
J	(Jonckheere)
*****	Avoid the usage of J, prefer Jonckheere
Origin	of the Acronym: L = Found in the literature
Details on Acronym: J
J	(Jansky (flux density))
*****	Avoid the usage of J, prefer 1Jy
Origin	of the Acronym: L = Found in the literature
Details on Acronym: J
J	(Jackson thesis)
*****	Avoid the usage of J, prefer [WCB96]
Origin	of the Acronym: L (1996ApJS..106....1W)
Details on Acronym: J1-
J1-	(Johnson, 1st list) (Not yet in Simbad)
*****	Avoid the usage of J1-, prefer [J55]
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: J1-
J1-	(Jones ?, 1st list)
*****	Avoid the usage of J1-, prefer [HJS91]
Origin	of the Acronym: L (1995ApJS..101..117K)
Details on Acronym: J2-
J2-	(Johnson, list 2) (Not yet in Simbad)
*****	Avoid the usage of J2-, prefer [J56]
Details on Acronym: J2-
J2-	(Jones ?, list 2)
*****	Avoid the usage of J2-, prefer [GJH92]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [J2003]
[J2003]	(Jones, 2003) (Not yet in Simbad)
Write:	<<[J2003] CN>> <<[J2003] FN>>
N:	6+3
Object:	* (SIMBAD class: Star)
Note:	Polarimetry at 1.65mi.m of stars shining in the GF 9 core (format CN) and GF 9 filament (format FN).
in source:	GF 9
Ref:	=2003AJ....125.3208J
by	JONES T.J.
	Astron. J., 125, 3208-3212 (2003)
	Grain alignment and the magnetic field geometry in the filamentary dark cloud GF 9.
o	Table 1: <[J2003] AN> (Nos C1-C6, F1-F3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [J2008]
[J2008]	(Jackson, 2008) (Not yet in Simbad)
Write:	<<[J2008] +S.ssss+S.sss>> <<[J2008] +S.sss+S.sss>> <<[J2008] +S.sss+S.ssss>>
N:	4+4
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Ref:	=2008MNRAS.389.1311J
by	JACKSON N.
	Mon. Not. R. Astron. Soc., 389, 1311-1318 (2008)
	Gravitational lenses and lens candidates identified from the COSMOS field.
o	Fig. 1: Candidate lens systems are not in Simbad (incomplete COSMOS identification).
o	Table 1: <[J2008] +S.ssss+S.sss> N=1, <[J2008] +S.sss+S.sss> N=3. Table 2: <[J2008] +S.sss+S.ssss> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [J55]
[J55]	(Johnson)= (J1-) (Not yet in Simbad)
Write:	<<[J55] NNN>>
N:	152
Object:	HII + RFN (SIMBAD class: ISM = Interstellar Medium Object)
Note:	152 objects among which 36 are new PN, also named 'PN YM NN' (Nos 1-36) (see YM)
Ref:	=1955ApJ...121..604J
by	JOHNSON H.M.
	Astrophys. J., 121, 604-610 (1955)
	Symmetric galactic nebulae.
o	Table 1: <[J55] NNN> (Nos 1-152), among which 36 are cross-id. with <PN YM NN> (Nos 1-36)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [J56]
[J56]	(Johnson)= (J2-) (Not yet in Simbad)
Write:	<<[J56] NN>>
N:	32
Object:	HII + RFN (SIMBAD class: ISM = Interstellar Medium Object)
Note:	32 objects among which 11 are new PN, also named 'PN YM NN' (Nos 37-47) (See YM)
Ref:	=1956ApJ...124...90J
by	JOHNSON H.M.
	Astrophys. J., 124, 90-92 (1956)
	Symmetric galactic nebulae. II.
o	Table 1: <[J56] NN> (Nos 1-32), among which 11 are cross-id. with <PN YM NN> (Nos 37-47)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [J76]
[J76]	(Johnson, 1976)
Write:	<<[J76] BHHMMSS.s+DDMMSS>>
N:	16
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Green Bank Observations. N=16 radio-sources in 9 Globular Clusters.
in source:	NGC 5024 = M 53
in source:	NGC 5272 = M 3
in source:	NGC 5904 = M 5
in source:	NGC 6205 = M 13
in source:	NGC 6440
in source:	NGC 6624
in source:	NGC 6864 = M 75
in source:	NGC 7078 = M 15
in source:	NGC 7089 = M 2
Ref:	=1976ApJ...208..706J
by	JOHNSON H.M.
	Astrophys. J., 208, 706-708 (1976)
	Radio sources in the field of globular clusters.
o	Table 1: <[J76] BHHMMSS.s+DDMMSS> N=16.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [J79]
[J79]	(Jacoby, 1979)= (J)
Write:	<<[J79] N>>
N:	4
Object:	Knot (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	Nuclear components of PN A66 30, sometime found with a format 'JN' (Jacoby) or a format 'KN' (Knot)
in source:	PN A66 30
Ref:	=1979PASP...91..754J
by	JACOBY G.H.
	Publ. Astron. Soc. Pac., 91, 754-760 (1979)
	Unusual structure in the planetary nebulae Abell 30 and Abell 78.
o	The companion star is WDS J08469+1753B.
o	Table II: <[J79] N> (Nos 1-4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [J80]
[J80]	(Johansson, 1980)
Write:	<<[J80] F-NNN>>
N:	341+197+170+210+169
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Danish 50cm and ESO 50cm telescope photoelectric UBV observations. UBV available, no coordinates only finding charts. Field 1: l=291.0, b=-0.1 Field 2: l=294.2, b=-1.8 Field 3: l=299.6, b=-1.8 Field 4: l=307.1, b=-2.1 Field 5: l=327.9, b=+1.8
Ref:	=1980A&AS...41...43J
by	JOHANSSON K.L.V.
	Astron. Astrophys., Suppl. Ser., 41, 43-66 (1980)
	Colour excess and stellar distribution in five selected directions of the Milky Way in Carina, Crux, Centaurus and Norma.
o	Main catalogue: <[J80] F-NNN> (Nos 1-1 to 1-341, 2-1 to 2-197, 3-1 to 3-170, 4-1 to 4-210, 5-1 to 5-169).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [J83]
[J83]	(Jagers, 1983)
Write:	<<[J83] 3C 130A>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio observations of two other double sources besides 3C 130, the northernmost is designed as '3C 130A', the southern one '3C 130B'.
Ref:	=1983A&A...125..172J
by	JAGERS W.J.
	Astron. Astrophys., 125, 172-174 (1983)
	The cluster around 3C 130.
o	Table 2: <[J83] 3C 130A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [J94]
[J94]	(Jonch-Sorensen, 1994)
Write:	<<[J94] FN-N>>
N:	22
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Table 5: 'zero point stars' in 6 fields (Nos F2, and F4 to F8)
Ref:	=1994A&AS..108..403J
by	JONCH-SORENSEN H.
	Astron. Astrophys., Suppl. Ser., 108, 403-408 (1994)
	CCD uvbyβ photometry of faint stars. I. Observations and reductions.
o	Table 5: <[J94] FN-N> N=22
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [J96]
[J96]	(Janulis, 1996)
Write:	<<[J96] NN>>
N:	63
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	SA 57-
Ref:	=1996BaltA...5..149J
by	JANULIS R.
	Baltic Astronomy, 5, 149-156 (1996)
	Vilnius photometry of stars in the area of SA 57.
o	Table 1: <[J96] NN> (Nos 1-63)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JA2003]
[JA2003]	(Jones+Amini, 2003) (Not yet in Simbad)
Write:	<<[JA2003] WN>> <<[JA2003] WNN>> <<[JA2003] Central Cluster N>> <<[JA2003] Central Cluster Neb NN>>
N:	8+8+9+13
Object:	* + Nebula (SIMBAD class: Star)
Note:	Study of DR 21 Central Cluster and Lobes East and West. Format 'WN' for stars in each lobe. Format 'WAN' where the letter N stands for Nebulosties in each lobe. Format 'Central Cluster N' for stars in the Central Cluster. Format 'Central Cluster Neb NN' for Nebulosties in the Central Cluster.
in source:	DR 21
Ref:	=2003AJ....125.1418J
by	JONES T.J. , AMINI H.
	Astron. J., 125, 1418-1425 (2003)
	The magnetic field geometry in DR 21.
o	<NAME DR 21 Central Cluster>. Table 2: <[JA2003] WN> (Nos E1-E5, W1-W3). Table 3: <[JA2003] WAN> (Nos EN1-EN5, WN1-WN3). Table 4: <[JA2003] Central Cluster N> (Nos 1-9). Table 5: <[JA2003] Central Cluster Neb NN> (Nos 1-13).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JAB78]
[JAB78]	(Jernican+Apparao+Bradt+, 1978)
Write:	<<[JAB78] 2S HHMM+DDd NN>>
N:	164
Object:	* (SIMBAD class: Star)
Note:	Finding charts
Ref:	=1978Natur.272..701J
by	JERNIGAN J.G. , APPARAO K.M.V., BRADT H.V., DOXSEY R.E., DOWER R.G., McCLINTOCK J.E.
	Nature, 272, 701-704 (1978)
	Positions of galactic X-ray sources : -20<lII<+6.
o	2S 1758-250 NN = [KOS70] GX 5-1 NN
o	Fig 2: <[JAB78] 2S 1702-363 NN> (Nos 1-10), <[JAB78] 2S 1702-429 NN> (Nos 1-37), <[JAB78] 2S 1705-440 N> (Nos 1-5), <[JAB78] 2S 1715-321 NN> (Nos 1-38), <[JAB78] 2S 1742-294 N> (Nos 1-8), <[JAB78] 2S 1755-338 NN> (Nos 1-27), <[JAB78] 2S 1803-245 NN> (Nos 1-29)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Jacoby
Jacoby	(Jacoby) (Not yet in Simbad)
Write:	<<Jacoby N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	The PN is found as 'Jacoby 1' in 1996ApJS..107..255T, = PN G85.4+46.4
Ref:	=1995AJ....110.1285J
by	JACOBY G.H. , VAN DE STEENE G.
	Astron. J., 110, 1285-1291 (1995)
	Identification of an old planetary nebula around the PG 1159 star: PG 1520+525.
o	The PN is PN G85.4+46.4 in SIMBAD. RX J2117+34 = RX J2117.1+3412
o	<Jacoby N> (No. 1).
Origin	of the Acronym: L (1996ApJS..107..255T)
Details on Acronym: Jacoby
Jacoby	(Jacoby)= (J)
Write:	<<Jacoby LMC NN>> <<Jacoby SMC NN>>
N:	41+27
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Table 2B: format LMC NN, (Nos 1-41), PN in the LMC. Table 2A: format SMC NN, (Nos 1-27), PN in the SMC. Identif. charts.
in source:	Magellanic Clouds:LMC = LMC
in source:	Magellanic Clouds:SMC = SMC
Ref:	=1980ApJS...42....1J
by	JACOBY G.H.
	Astrophys. J., Suppl. Ser., 42, 1-18 (1980)
	The luminosity function for planetary nebulae and the number of planetary nebulae in local group galaxies.
o	Table 2A: <Jacoby SMC NN> (Nos 1-27). Table 2B: <Jacoby LMC NN> (Nos 1-41).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: JaFu
JaFu	(Jacoby+Fullton)
Write:	<<PN JaFu N>>
N:	2
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	N=2 PN from a private communication of Jacoby.
Ref:	=1997AJ....114.2611J
by	JACOBY G.H. , MORSE J.A., FULLTON L.K., KWITTER K.B., HENRY R.B.C.
	Astron. J., 114, 2611-2625 (1997)
	Planetary nebulae in the globular clusters Pal 6 and NGC 6441.
o	(Erratum) + erratum AJ 115, p. 1688.
o	<PN JaFu N> (Nos 1-2)
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [JAP2011]
[JAP2011]	(Jacobs+Aguirre+Parsons+, 2011)
Write:	<<[JAP2011] JDDD.dd+DD.dd>>
N:	480
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Precision Array for Probing the Epoch of Reionization (PAPER) 145GHz observations of N=480 sources. Use of the 408MHz Molonglo Reference Catalog (MRC).
Ref:	=2011ApJ...734L..34J
by	JACOBS D.C. , AGUIRRE J.E., PARSONS A.R., POBER J.C., BRADLEY R.F., CARILLI C.L., GUGLIUCCI N.E., MANLEY J.R., VAN DER MERWE C., MOORE D.F., PARASHARE C.R.
	Astrophys. J., 734L, 34 (2011)
	New 145 MHz source measurements by PAPER in the southern sky.
o	Table 2: <[JAP2011] JDDD.dd+DD.dd> N=480.
=E=	Catalogue in electronic form as <J/ApJ/734/L34/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JaSt
JaSt	(Jacoby+van de Steene)
Write:	<<JaSt NN>>
N:	98
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	See also JaSt2
Ref:	=2001A&A...373..536V
by	VAN DE STEENE G.C. , JACOBY G.H.
	Astron. Astrophys., 373, 536-541 (2001)
	Radio observations of new galactic bulge planetary nebulae.
o	Table 1: <JaSt NN> N=64 among (Nos 1-98).
Ref:	=2001RMxAA..37..115K
by	KIMESWENGER S.
	Rev. Mex. Astron. Astrofis., 37, 115-145 (2001)
	Optical coordinates of southern planetary nebulae.
o	Table 3: IRAS 18150-2550 misprint for ?
o	Table 2: <JaSt NN> (Nos 39, 43, 72) added.
Ref:	=2004A&A...419..563J
by	JACOBY G.H. , VAN DE STEENE G.
	Astron. Astrophys., 419, 563-582 (2004)
	Planetary nebulae near the Galactic Center: Identifications.
o	Table 2: <JaSt NN> (Nos 1-98). Table 3: <JaSt2 NN> (Nos 1-20).
=E=	Catalogue in electronic form as J/A+A/373/536
=E=	Catalogue in electronic form as J/other/RMxAA/37.115
=E=	Catalogue in electronic form as J/A+A/419/563
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: JaSt2
JaSt2	(Jacoby+van de Steene, list 2)
Write:	<<JaSt2 NN>>
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	New PNs discovered in the H-alpha survey 2Wat the WIYN telescope. Finding charts. See also JaSt
Ref:	=2004A&A...419..563J
by	JACOBY G.H. , VAN DE STEENE G.
	Astron. Astrophys., 419, 563-582 (2004)
	Planetary nebulae near the Galactic Center: Identifications.
o	Table 2: <JaSt NN> (Nos 1-98). Table 3: <JaSt2 NN> (Nos 1-20).
=E=	Catalogue in electronic form as J/A+A/419/563
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: JB
JB	(J. Breysacher)
*****	Avoid the usage of JB, prefer Brey
Details on Acronym: JB
JB	(Johansson+Bergvall)
Write:	<<JB {a\|b} NN>> <<JB a NN-N>>
N:	59+33+38
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	1990A&AS...86..167J, Table 1a: N=59 interacting galaxies, format 'a NN' in SIMBAD. 1990A&AS...86..167J, Table 1b: N=38 isolated galaxies, format 'b NN' in SIMBAD. 1997A&AS..126....3H, Table 1: N=33 components of some interacting galaxies, format 'a NN-1' and 'a NN-2' in SIMBAD, format 'NN-N' in the paper.
Ref:	=1990A&AS...86..167J
by	JOHANSSON L. , BERGVALL N.
	Astron. Astrophys., Suppl. Ser., 86, 167-None (1990)
	A study of a complete sample of interacting galaxies. I. Presentation of the sample and the UBVRIJHK photometry.
o	Table 1a: <JB a NN> (Nos 1-59). Table 1b: <JB b NN> (Nos 1-38).
Ref:	=1997A&AS..126....3H
by	HORELLOU C. , BOOTH R.
	Astron. Astrophys., Suppl. Ser., 126, 3-13 (1997)
	CO and HI in a southern sample of interacting galaxies. I. The data.
o	Table 1: <JB a NN-N> N=33
Origin	of the Acronym: A (1997A&AS..126....3H)
Details on Acronym: [JB2000]
[JB2000]	(Jimenez-Vicente+Battaner, 2000) (Not yet in Simbad)
Write:	<<[JB2000] A>>
N:	8
Object:	Region (SIMBAD class: Region = Region defined in the Sky)
Note:	Fig.5, Table 3: (Nos A-H), high residual velocity regions.
in source:	NGC 5668
Ref:	=2000A&A...358..812J
by	JIMENEZ-VICENTE J. , BATTANER E.
	Astron. Astrophys., 358, 812-818 (2000)
	Vertical motions in the disk of NGC 5668 as seen with optical Fabry-Perot spectroscopy.
o	Fig.5, Table 3: <[JB2000] A> (Nos A-H).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JB2001]
[JB2001]	(Jones+Bland-Hawthorn, 2001) (Not yet in Simbad)
Write:	<<[JB2001] NNN.NN>>
N:	7
Object:	G (SIMBAD class: Galaxy)
Note:	Sample selection of 7 galaxies.
Ref:	=2001ApJ...550..593J
by	JONES D.H. , BLAND-HAWTHORN J.
	Astrophys. J., 550, 593-611 (2001)
	The Taurus tunable filter field galaxy survey: sample selection and narrowband number counts.
o	Fig.4: <[JB2001] NNN.NN> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JB2006]
[JB2006]	(Johnstone+Bally, 2006)= (SMM)
Write:	<<[JB2006] SMM JHHMMmm+DDMMm>> <<[JB2006] NN>>
N:	71
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	JCMT SCUBA observations of Ori A molecular cloud.
in source:	NAME Ori A
Ref:	=2006ApJ...653..383J
by	JOHNSTONE D. , BALLY J.
	Astrophys. J., 653, 383-397 (2006)
	Large-area mapping at 850 µm. V. Analysis of the clump distribution in the Orion A South molecular cloud.
o	Table 1: <[JB2006] SMM JHHMMmm+DDMMm> = <[JB2006] NN> (Nos 1-71). Paragr. 4.2.2: <OMC N> (No. 5) added.
=E=	Catalogue in electronic form as J/ApJ/653/383
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JB2015]
[JB2015]	(Jones+Braiding, 2015)
Write:	<<[JB2015] A>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA observations at 1332, 1844 and 2868MHz of N=3 strong peaks in the star-forming region PMN J1452-5910 = IRAS 14482-5857.
in source:	PMN J1452-5910
Ref:	=2015AJ....149...70J
by	JONES D.I. , BRAIDING C.R.
	Astron. J., 149, 70 (2015)
	Discovery of luminous star formation in PMN 1452-5910/IRAS 14482-5857: the pterodactyl nebula.
o	Fig. 2, Table 1: <[JB2015] A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JBA2003]
[JBA2003]	(Johnson+Best+Almaini, 2003)
Write:	<<[JBA2003] NN>>
N:	47
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of ClG 1054.4-0321.
in source:	1E 1054.4-0321 = ClG 1054-0321
Ref:	=2003MNRAS.343..924J
by	JOHNSON O. , BEST P.N., ALMAINI O.
	Mon. Not. R. Astron. Soc., 343, 924-932 (2003)
	The content of active galactic nuclei in the z = 0.83 cluster MS 1054-0321.
o	Table 1: <[JBA2003] NN> (Nos 1-47).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JBC2011]
[JBC2011]	(Jenkins+Brandt+Colbert+, 2011)
Write:	<<[JBC2011] NN>>
N:	28
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra and XMM-Newton X-ray observations of NGC 1672.
in source:	NGC 1672
Ref:	=2011ApJ...734...33J
by	JENKINS L.P. , BRANDT W.N., COLBERT E.J.M., KORIBALSKI B., KUNTZ K.D., LEVAN A.J., OJHA R., ROBERTS T.P., WARD M.J., ZEZAS A.
	Astrophys. J., 734, 33 (2011)
	Investigating the nuclear activity of barred spiral galaxies: the case of NGC 1672.
o	Table 1: <[JBC2011] NN> (Nos 1-28).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JBD2005]
[JBD2005]	(Jorgensen+Bergmann+Davies+, 2005)
Write:	<<[JBD2005] NNNN>>
N:	44
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Gemini GMOS-N observations of the galaxy cluster RX J0152.7-1357.
in source:	RX J0152.7-1357 = ClG J0152-1357
Ref:	=2005AJ....129.1249J
by	JORGENSEN I. , BERGMANN M., DAVIES R., BARR J., TAKAMIYA M., CRAMPTON D.
	Astron. J., 129, 1249-1286 (2005)
	RX J0152.7-1357: stellar populations in an X-ray luminous galaxy cluster at z = 0.83.
o	Tables 6, 10: <[JBD2005] NNNN> N=44 among (Nos 103-2087).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JBD79]
[JBD79]	(Johnston+Bradt+Doxsey, 1979)
Write:	<<[JBD79] LMC X-2 A>> <<[JBD79] LMC X-3 A>> <<[JBD79] H 0544-665 NN>>
N:	7+4+24
Object:	* (SIMBAD class: Star)
Note:	HEAO 1 observations. Fig.5: N=7 * in the field of LMC X-2, (Nos A-G) and N=4 * in the field of LMC X-3, (Nos A-D). Fig.6: N=24 * in the field of H 0544-665, (Nos 1-24). Finding charts
in source:	Magellanic Clouds:LMC:LMC X-2 = LMC X-2
in source:	Magellanic Clouds:LMC:LMC X-3 = LMC X-3
in source:	H 0544-665
Ref:	=1979ApJ...233..514J
by	JOHNSTON M.D. , BRADT H.V., DOXSEY R.E.
	Astrophys. J., 233, 514-523 (1979)
	A six-month X-ray survey of the Large Magellanic Cloud with the HEAO 1 scanning modulation collimator.
o	* 15 and 22 in LMC X-2 = [CCH78] LMC X-2 15 and 22. * WP in LMC X-3 = [WP75] 8
o	Fig.5: <[JBD79] LMC X-2 A> (Nos A-G), <[JBD79] LMC X-3 A> (Nos A-D). Fig.6: <[JBD79] H 0544-665 NN> (Nos 1-24).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JBF
JBF	(Jodrell Bank Flat-spectrum)
Write:	<<JBF NNN>>
N:	117
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Jodrell Bank Flat-spectrum sample: VLA 4.86GHz observations of flat-spectrum radio sources.
Ref:	=2007MNRAS.377..430M
by	McKEAN J.P. , BROWNE I.W.A., JACKSON N.J., FASSNACHT C.D., HELBIG P.
	Mon. Not. R. Astron. Soc., 377, 430-440 (2007)
	The Cosmic Lens All-Sky Survey parent population - I. Sample selection and number counts.
o	Table 3: <JBF NNN> (Nos 1-117).
=E=	Catalogue in electronic form as J/MNRAS/377/430
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [JBF2000]
[JBF2000]	(Jerjen+Binggeli+Freeman, 2000)
Write:	<<[JBF2000] Cen A-dEN>> <<[JBF2000] Scl-dEN>> <<[JBF2000] HHMMSS.s+DDMMSS>>
N:	5+1+2
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=5+1 dwarf elliptical galaxies ('dE' in the format) in Cen A and Sculptor groups of galaxies. N=2 candidates in Scl format 'HHMMSS.s+ DDMMSS'.
in source:	NAME CEN A GROUP
in source:	NAME SCL GROUP
Ref:	=2000AJ....119..593J
by	JERJEN H. , BINGGELI B., FREEMAN K.C.
	Astron. J., 119, 593-608 (2000)
	Surface BR photometry of newly discovered dwarf elliptical galaxies in the nearby Sculptor and Centaurus A groups.
o	T.1 : SGC 1319.1-4216 = SGC 131907-4216.5, SC22 and Cen 8 = [CFC97] Sc 22 and [CFC97] Cen 8.
o	Fig.1, Table 1: <[JBF2000] Cen A-dEN> (Nos dE1 to dE5), <[JBF2000] Scl-dEN> (No. dE1). p.594: <[JBF2000] HHMMSS.s+ DDMMSS> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JBF2005]
[JBF2005]	(Jakobsson+Bjornsson+Fynbo+, 2005) (Not yet in Simbad)
Write:	<<[JBF2005] S1004-N>> <<[JBF2005] S0226-N>>
N:	7+5
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=7+5 candidate LEGOs (Ly-alpha Emitting Galaxy-building Object) in the field of GRB 021004 (1004 in the format) and GRB 030226 (0226 in the format) respectively. See also [FJM2003], [FMT2002], LEGO.
Ref:	=2005MNRAS.362..245J
by	JAKOBSSON P. , BJORNSSON G., FYNBO J.P.U., JOHANNESSON G., HJORTH J., THOMSEN B., MOLLER P., WATSON D., JENSEN B.L., OSTLIN G., GOROSABEL J., GUDMUNDSSON E.H.
	Mon. Not. R. Astron. Soc., 362, 245-251 (2005)
	Ly+ and ultraviolet emission from high-redshift γ-ray burst hosts: to what extent do γ-ray bursts trace star formation ?
o	Standard star BD +28 not identified, incomplete format.
o	Fig.2, Table 2: <[JBF2005] S1004-N> (Nos 1 to 7). Fig.2, Table 3: <[JBF2005] S0226-N> (Nos 1 to 5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JBF2020]
[JBF2020]	(Jones+Bethermin+Fudamoto+, 2020)
Write:	<<[JBF2020] DEIMOS COSMOS 818760 C>> <<[JBF2020] DEIMOS COSMOS 818760 W>>
N:	3
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ALMA band 7 [CII] observations of N=3 sources in the field of COSMOS2015 818760 (= DEIMOS COSMOS 818760).
Ref:	=2020MNRAS.491L..18J
by	JONES G.C. , BETHERMIN M., FUDAMOTO Y., GINOLFI M., CAPAK P., CASSATA P., FAISST A., LE FEVRE O., SCHAERER D., SILVERMAN J.D., YAN L., BARDELLI S., BOQUIEN M., CIMATTI A., DESSAUGES-ZAVADSKY M., GIAVALISCO M., GRUPPIONI C., IBAR E., KHUSANOVA Y., KOEKEMOER A.M., LEMAUX B.C., LOIACONO F., MAIOLINO R., OESCH P.A., POZZI F., RIECHERS D., RODIGHIERO G., TALIA M., VALLINI L., VERGANI D., ZAMORANI G., ZUCCA E.
	Mon. Not. R. Astron. Soc., 491L, 18 (2020)
	The ALPINE-ALMA [C II] Survey: a triple merger at z 4.56.
o	Fig. 1, Table 1: <[JBF2020] DEIMOS COSMOS 818760 A> (Nos C, E, W).
o	DEIMOS COSMOS 818760 is COSMOS2015 818760 in SIMBAD. J0158+0133 (calibrator) is a probable misprint for J1058+0133.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JBJ2014]
[JBJ2014]	(Joshi+Balona+Joshi+, 2014)
Write:	<<[JBJ2014] NNNN>>
N:	2393
Object:	* (SIMBAD class: Star)
Note:	1-m Sampurnanand telescope (Nainital, India) UBVRI photometry of N=2393 stars in the field of the open cluster NGC 559.
in source:	NGC 559
Ref:	=2014MNRAS.437..804J
by	JOSHI Y.C. , BALONA L.A., JOSHI S., KUMAR B.
	Mon. Not. R. Astron. Soc., 437, 804-815 (2014)
	Photometric study of the open cluster - II. Stellar population and dynamical evolution in NGC 559.
o	Table 4: <[JBJ2014] NNNN> (Nos 1-2393).
=E=	Catalogue in electronic form as J/MNRAS/437/804
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JBK93]
[JBK93]	(Juan+Bachiller+Kompe+, 1993)
Write:	<<[JBK93] AN>>
N:	6
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=6 NH3 clumps in LDN 1455.
in source:	LDN 1455
Ref:	=1993A&A...270..432J
by	JUAN J. , BACHILLER R., KOMPE C., MARTIN-PINTADO J.
	Astron. Astrophys., 270, 432-443 (1993)
	High density structure of the L 1455 dark cloud.
o	Fig.6, Table 4: <[JBK93] AN> (Nos A1-A2, B-E).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JBL2014]
[JBL2014]	(Johnston+Beuther+Linz+, 2014)
Write:	<<[JBL2014] NN>>
N:	36
Object:	(mm) (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	SMA 1.3mm and IRAM 30m observations of N=36 dust cores within the massive Galactic center cloud G0.253+0.016.
in source:	GAL 000.253+00.016
Ref:	=2014A&A...568A..56J
by	JOHNSTON K.G. , BEUTHER H., LINZ H., SCHMIEDEKE A., RAGAN S.E., HENNING Th.
	Astron. Astrophys., 568A, 56-56 (2014)
	The dynamics and star-forming potential of the massive Galactic centre cloud G0.253+0.016.
o	Table 2: <[JBL2014] NN> (Nos 1-36).
=E=	Catalogue in electronic form as <J/A+A/568/A56/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JBM2010]
[JBM2010]	(James+Barnes+Meibom+, 2010)
Write:	<<[JBM2010] FF NNNN>>
N:	55
Object:	V* (SIMBAD class: Variable* = Variable Star)
Note:	WIYN 0.9m telescope observations of the open cluster NGC 1039.
in source:	NGC 1039
Ref:	=2010A&A...515A.100J
by	JAMES D.J. , BARNES S.A., MEIBOM S., LOCKWOOD G.W., LEVINE S.E., DELIYANNIS C., PLATAIS I., STEINHAUER A., HURLEY B.K.
	Astron. Astrophys., 515A, 100-100 (2010)
	New rotation periods in the open cluster NGC 1039 (M34), and a derivation of its gyrochronology age.
o	Tables 2-3, A.1: <[JBM2010] FF NNNN> N=55 among (Nos F3 71 to F3 2310, F4 136 to F4 2226).
=E=	Catalogue in electronic form as J/A+A/515/A100
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JBM2013]
[JBM2013]	(Janes+Barnes+Meibom+, 2013)
Write:	<<[JBM2013] NNNNN>>
N:	10674
Object:	* (SIMBAD class: Star)
Note:	Lowell Observatory 1.08m Hall and 1.83m Perkins telescope observations of N=10674 stars in the field of the open star cluster NGC 6811.
in source:	NGC 6811
Ref:	=2013AJ....145....7J
by	JANES K. , BARNES S.A., MEIBOM S., HOQ S.
	Astron. J., 145, 7 (2013)
	NGC 6811: an intermediate-age cluster in the Kepler field.
o	Table 3: <[JBM2013] NNNNN> (Nos 1-10674).
=E=	Catalogue in electronic form as <J/AJ/145/7/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JBN2006]
[JBN2006]	(Jonker+Bassa+Nelemans+, 2006)
Write:	<<[JBN2006] Star A>>
N:	4
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS2 observations of 1H 1905+000. N=4 stars near 1H 1905+000.
Ref:	=2006MNRAS.368.1803J
by	JONKER P.G. , BASSA C.G., NELEMANS G., JUETT A.M., BROWN E.F., CHAKRABARTY D.
	Mon. Not. R. Astron. Soc., 368, 1803-1810 (2006)
	The neutron star soft X-ray transient 1H 1905+000 in quiescence.
o	Fig.2: <[JBN2006] Star A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JBN2011]
[JBN2011]	(Jonker+Bassa+Nelemans+, 2011)= (GBS)
Write:	<<[JBN2011] NNNN>>
N:	1234
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	N=1234 X-ray sources from the Chandra Galactic Bulge Survey. See also CXOGBS.
Ref:	=2011ApJS..194...18J
by	JONKER P.G. , BASSA C.G., NELEMANS G., STEEGHS D., TORRES M.A.P., MACCARONE T.J., HYNES R.I., GREISS S., CLEM J., DIEBALL A., MIKLES V.J., BRITT C.T., GOSSEN L., COLLAZZI A.C., WIJNANDS R., IN'T ZAND J.J.M., MENDEZ M., REA N., KUULKERS E., RATTI E.M., VAN HAAFTEN L.M., HEINKE C., OZEL F., GROOT P.J., VERBUNT F.
	Astrophys. J., Suppl. Ser., 194, 18 (2011)
	The Galactic Bulge Survey: outline and X-ray observations.
o	Table 3, col(1): <CXOGBS JHHMMSS.s+DDMMSS> N=1234 = Table 3, col(2): <[JBN2011] NNNN> (Nos 1-1234).
=E=	Catalogue in electronic form as J/ApJS/194/18
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JBO2001]
[JBO2001]	(Jain+Bailyn+Orosz+, 2001)
Write:	<<[JBO2001] A>>
N:	4
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=4 calibration standards in the field of XTE J1550-564. Finding chart Fig.2.
Ref:	=2001ApJ...546.1086J
by	JAIN R.K. , BAILYN C.D., OROSZ J.A., McCLINTOCK J.E., SOBCZAK G.J., REMILLARD R.A.
	Astrophys. J., 546, 1086-1097 (2001)
	Optical observations of the black hole candidate XTE J1550-564 during reflare and quiescence.
o	Table 2, Fig.2: <[JBO2001] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JBP2003]
[JBP2003]	(Jackson+Beswick+Pedlar+, 2003)
Write:	<<[JBP2003] Star N>> <<[JBP2003] WW Arm>> <<[JBP2003] WW Lobe>> <<[JBP2003] WW Jet>> <<[JBP2003] NE Jet A>>
N:	4+8
Object:	* + (Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	MERLIN and HST observations of the central region of 3C 305 radio galaxy. N=4 standard stars in the field of 3C 305. Radio components of 3C 305.
in source:	3C 305
Ref:	=2003MNRAS.338..643J
by	JACKSON N. , BESWICK R., PEDLAR A., COLE G.H., SPARKS W.B., LEAHY J.P., AXON D.J., HOLLOWAY A.J.
	Mon. Not. R. Astron. Soc., 338, 643-654 (2003)
	Observations of the neutral gas and dust in the radio galaxy 3C 305.
o	Table 2: <[JBP2003] Star N> (Nos 1-4). Table 3: <[JBP2003] WW Arm> (Nos NE, SW), <[JBP2003] WW Lobe> (Nos NE, SW), <[JBP2003] WW Jet> (Nos NE, SW), <[JBP2003] NE Jet A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JBT2003]
[JBT2003]	(Jenkins+Bowen+Tripp+, 2003)
Write:	<<[JBT2003] GNNN>> <<[JBT2003] SNNN>> <<[JBT2003] QSO J2155-0922 abs N.NNNNN>>
N:	7+4+7
Object:	G + * (SIMBAD class: UV = UV-emission Source)
Stat:	is completely incorporated in Simbad
Note:	FUSE observations of the field of PHL 1811. The numbering in the format is from a catalog of objects generated by SExtractor from an image from the MDM 1.3m McGraw-Hill telescope. 7 absorbers are seen in the spectrum of PHL 1811 = QSO J2155-0922.
Ref:	=2003AJ....125.2824J
by	JENKINS E.B. , BOWEN D.V., TRIPP T.M., SEMBACH K.R., LEIGHLY K.M., HALPERN J.P., LAUROESCH J.T.
	Astron. J., 125, 2824-2841 (2003)
	Absorption-line systems and galaxies in front of the second-brightest quasar, PHL 1811.
o	Table 4: <[JBT2003] QSO J2155-0922 abs N.NNNNN> N=7. Table 7: <[JBT2003] ANNN> N=7 among (Nos G82-G209), N=4 among (Nos S133-S144).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JBT2005]
[JBT2005]	(Jenkins+Bowen+Tripp+, 2005) (Not yet in Simbad)
Write:	<<[JBT2005] AN>>
N:	3
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Structure of the QSO PHL 1811: N=2 nebulous cores A1 and A2, N=1 arc of emission A3.
in source:	PHL 1811 = QSO J2155-0922
Ref:	=2005ApJ...623..767J
by	JENKINS E.B. , BOWEN D.V., TRIPP T.M., SEMBACH K.R.
	Astrophys. J., 623, 767-794 (2005)
	A near-solar metallicity, nitrogen-deficient Lyman limit absorber associated with two S0 galaxies.
o	note 23: Q1409+0950 is a misprint for QSO 1409+0930.
o	Fig.11: <[JBT2005] AN> (Nos A1-A3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JBV2003]
[JBV2003]	(Johnstone+Boonman+Van Dishoeck, 2003)
Write:	<<[JBV2003] PDR1-OMC1>> <<[JBV2003] SK1-OMC3>>
N:	1+1
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	N=2 new smm bright regions in Orion, PDR1 (PhotoDissociation Region) in OMC 1, SK1 (Strong shock front) in OMC 3, compiled from 1999ApJ...510L..49J.
in source:	OMC:OMC 1 = OMC 1
in source:	OMC:OMC 3 = OMC 3
Ref:	=2003A&A...412..157J
by	JOHNSTONE D. , BOONMAN A.M.S., VAN DISHOECK E.F.
	Astron. Astrophys., 412, 157-174 (2003)
	Astrochemistry of sub-millimeter sources in Orion. Studying the variations of molecular tracers with changing physical conditions.
o	Table 1: MMS objects = [CRW97] OMC-3 MMS N, FIR4 = [MWZ90] OMC-2 FIR 4, and NAME NGC 2071 IR
o	Table 1: <[JBV2003] PDR1-OMC1> N=1, <[JBV2003] SK1-OMC3> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JBZ2006]
[JBZ2006]	(Johnson+Best+Zaritsky+, 2006)
Write:	<<[JBZ2006] Cl JHHMM XNN>> <<[JBZ2006] JHHMMSS.ss+DDMMSS.s>> <<[JBZ2006] ClHHMM_NN>> (not recognised by Simbad, but found in literature)
N:	77+67+67+92+72+84
Object:	(X) + (Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of 3 clusters from the the ESO Distant Cluster Survey (EDisCS).
in source:	ClG J1216-1201
in source:	ClG J1054-1146
in source:	ClG J1040-1155
Ref:	=2006MNRAS.371.1777J
by	JOHNSON O. , BEST P., ZARITSKY D., CLOWE D., ARAGON-SALAMANCA A., HALLIDAY C., JABLONKA P., MILVANG-JENSEN B., PELLO R., POGGIANTI B.M., RUDNICK G., SAGLIA R., SIMARD L., WHITE S.
	Mon. Not. R. Astron. Soc., 371, 1777-1792 (2006)
	The X-ray properties of optically selected z > 0.6 clusters in the European Southern Observatory Distant Cluster Survey.
o	Table 1: Cl1054-1145 = ClG J1054-1146 in SIMBAD.
o	Table a1: <[JBZ2006] Cl J1216 XNN> (Nos 1-77). Table a2: <[JBZ2006] Cl J1054 XNN> (Nos 1-67). Table a3: <[JBZ2006] Cl J1040 XNN> (Nos 1-67). Tables b1-b3: <[JBZ2006] JHHMMSS.ss+DDMMSS.s> N=92+72+84.
=E=	Catalogue in electronic form as J/MNRAS/371/1777
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JC2013]
[JC2013]	(Jorgensen+Chiboucas, 2013)
Write:	<<[JC2013] MS0451.6-0305 NNNN>> <<[JC2013] RXJ1226.9+3332 NNNN>>
N:	70+119
Object:	G (SIMBAD class: Galaxy)
Note:	N=70+119 galaxies in the field of MS 0451.6-0305 and RX J1226.9+3332 galaxy clusters. Use of Gemini-North GMOS and HST ACS data.
in source:	ClG 0451.0-0305
in source:	RX J1226.0+3332
Ref:	=2013AJ....145...77J
by	JORGENSEN I. , CHIBOUCAS K.
	Astron. J., 145, 77 (2013)
	Stellar populations and evolution of early-type cluster galaxies: constraints from optical imaging and spectroscopy of z=0.5-0.9 galaxy clusters.
o	RXJ0157.2-1357 (Table 1), RXJ0152.7-0152 (p.11), RXJ0152.7-0305 (p.17) and RXJ0152.7-1257 (p.55) are misprints for RXJ0152.7-1357. MS0451.6-0307 (p.15) and MS0451.1-0306 (p.28) are misrpints for MS0451.6-0305. RXJ1226.9+3336 (p.9) and RXJ1226.6+3332 (p.20) are misprints for RXJ1226.9+3332.
o	Fig. 1, Tables 13, 15, 21, 22: <[JC2013] MS0451.6-0305 NNNN> N=70 among (Nos 12-3906). Fig. 2, Tables 14, 23, 24: <[JC2013] RXJ1226.9+3332 NNNN> N=119 among (Nos 18-1254).
=E=	Catalogue in electronic form as <J/AJ/145/77/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JC93]
[JC93]	(Jiang+Chen, 1993)
Write:	<<[JC93] 1-N>> <<[JC93] 2-NN>>
N:	5+15
Object:	V* + Em. G (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	Table I: format '1-N' (Nos 1-5), V* Table II: format '2-NN' (Nos 1-15), Em. G
Rem:	Finding charts
Ref:	=1993AcApS..13..378J
by	JIANG Z.-J. , CHEN J.-S.
	Acta Astrophys. Sinica, 13, 378-384 (1993)
	Computer automatic search for variable stars and emission line galaxies.
o	Table 1: <[JC93] 1-N> N=5. Table 2: <[JC93] 2-NN> N=15
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCB2001]
[JCB2001]	(Jeltema+Canizares+Bautz+, 2001)
Write:	<<[JCB2001] W Clump>> <<[JCB2001] JHHMMSS.s+DDMMSS.s>>
N:	2+3
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS-S observations of the cluster ClG 1054-0321 (1E 1054.5-0321). N=2 X-ray clumps (Nos W, W) and N=3 point sources designated by their coordinates 'JHHMMSS.s+DDMMSS.s'. See also [DVG98], [NA2000], [HFK2000].
in source:	1E 1054.4-0321 = ClG 1054-0321
Ref:	=2001ApJ...562..124J
by	JELTEMA T.E. , CANIZARES C.R., BAUTZ M.W., MALM M.R., DONAHUE M., GARMIRE G.P.
	Astrophys. J., 562, 124-132 (2001)
	Chandra X-ray observatory observation of the high-redshift cluster MS 1054-0321.
o	<[JCB2001] W Clump> (Nos E, W). <[JCB2001] JHHMMSS.s+DDMMSS.s> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCB2003]
[JCB2003]	(Jeltema+Canizares+Buote+, 2003)
Write:	<<[JCB2003] NN>>
N:	42
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of NGC 720.
in source:	NGC 720
Ref:	=2003ApJ...585..756J
by	JELTEMA T.E. , CANIZARES C.R., BUOTE D.A., GARMIRE G.P.
	Astrophys. J., 585, 756-766 (2003)
	X-ray source population in the elliptical galaxy NGC 720 with Chandra.
o	Table 2: <[JCB2003] NN> (Nos 1-42).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCB2007]
[JCB2007]	(Jin+Cao+Bian+, 2007)
Write:	<<[JCB2007] JHHMMSS.ss+DDMMSS.s>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Host galaxies of SN 2007H and SN 2007I.
Ref:	=2007IAUC.8798....1J
by	JIN C.C. , CAO Y., BIAN F.-Y., LOU Y.-Q., WANG X.F., WU Y., YANG Y., NEWTON J., PUCKETT T., LEE N., LI W., JOUBERT N., MADISON D.R., MOSTARDI R.
	IAUC, 8798, 1 (2007)
	Supernovae 2007G, 2007H, 2007I, 2007J, 2007K, 2007L, 2007M.
o	<[JCB2007] JHHMMSS.ss+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCB2017]
[JCB2017]	(Jorgensen+Chiboucas+Berkson+, 2017)
Write:	<<[JCB2017] A1689 NNNN>> <<[JCB2017] RXJHHMM NNNN>> <<[JCB2017] RXJ0027.6+2616 foreground group>>
N:	251
Object:	G + GrG (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Gemini GMOS-N and GMOS-S observations of N=251 galaxies in the field of N=4 galaxy clusters at z=0.19-0.45. Use of archival HST ACS imaging. See also [JCF2006], [JC2013] and [JCT2014].
Ref:	=2017AJ....154..251J
by	JORGENSEN I. , CHIBOUCAS K., BERKSON E., SMITH O., TAKAMIYA M., VILLAUME A.
	Astron. J., 154, 251-251 (2017)
	Galaxy populations in massive z = 0.2-0.9 clusters. I. Analysis of spectroscopy.
o	Misprints: 1E 0451.3-0306 => 1E 0451.6-0305; RXJ0152.7-1157 and RXJ0152.7-1347 => RXJ0152.7-1357; RXJ1226.9+2226 => RXJ1226.9+3332; RXJ1347.5+1145, RXJ1347.5-1345, RXJ1347.5-1347 and RXJ1347.5-1137 => RXJ1347.5-1145.
o	Table 8: <[JCB2017] A1689 NNNN> N=78 among (Nos 14-1164), <[JCB2017] RXJ0056 NNNN> N=66 among (Nos 2-1480), <[JCB2017] RXJ0027 NNNN> N=47 among (Nos 1-1187), <[JCB2017] RXJ1347 NNNN> N=60 among (Nos 75-1186). Text: [JCB2017] RXJ0027.6+2616 foreground group> N=1.
=E=	Catalogue in electronic form as J/AJ/154/251
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCC87]
[JCC87]	(Jennings+Cameron+Cudlip+, 1987)= (IRAS)
Write:	<<[JCC87] IRAS NAN>>
N:	9+8+2+2
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	IRAS CPC observations. IRAS 2A is found 1st in IAUS vol.178, p.31, Blake. Format 'IRAS NA' is sometimes found as 'IRAS Na'. IRAS 4A has 2 components 4A1 and 4A2. IRAS 4B has 2 components 4B1 and 4B2, sometimes found as 4BI and 4BII, or 4BW and 4BE respectively. 4A2 is found as 4A' and 4B2 as 4B' in 2001ApJ...562..770D. 4B2 is also named 4C in 1999ApJS..122..519C (not SIMBAD 4C first found in 1999ApJS..125..427R)
in source:	NGC 1333
Ref:	=1987MNRAS.226..461J
by	JENNINGS R.E. , CAMERON D.H.M., CUDLIP W., HIRST C.J.
	Mon. Not. R. Astron. Soc., 226, 461-471 (1987)
	IRAS observations of NGC 1333.
o	Table 1: cross-id. FIRSSE 42 not in SIMBAD. Table 2: IRAS found by coordinates.
o	Table 1: <[JCC87] IRAS N> (Nos 1-9)
Ref:	=1991ApJ...376L..17S
by	SANDELL G. , ASPIN C., DUNCAN W.D., RUSSELL A.P.G., ROBSON E.I.
	Astrophys. J., 376, 17-20 (1991)
	NGC 1333 IRAS 4 : a very young, low-luminosity binary system.
o	Table 1: H2O(C) and (D) = [HMR80] H2O(C) and (D)
o	Table 1: <[JCC87] IRAS NA> (Nos 4A, 4B)
Ref:	=1993BAAS...25.1367W
by	WOOTTEN A. , MANGUM J.
	Bull. American Astron. Soc., 25, 1367-None (1993)
	Coeval but separate star formation in NGC1333 IRAS4.
o	<[JCC87] IRAS NA> (No. 4C)
Ref:	=1996ApJ...473L..49B
by	BALLY J. , DEVINE D., REIPURTH B.
	Astrophys. J., 473, 49-54 (1996)
	A burst of Herbig-Haro flows in NGC 1333.
o	Table 3: IRAS f = IRAS 03262+3108
o	Table 2: <HH NNNA> (Nos 333-353). Table 3: <[SVS76] NGC 1333 NNA> (No. 13B). Table 3: <[JCC87] IRAS NA> (Nos 2B, 7A, 7B).
Ref:	=1999ApJ...525L.109G
by	GIRART J.M. , CRUTCHER R.M., RAO R.
	Astrophys. J., 525, 109-112 (1999)
	Detection of polarized CO emission from the molecular outflow in NGC 1333 IRAS 4A.
o	<[JCC87] IRAS NAN> (Nos 4A1-4A2).
Ref:	=1999ApJS..125..427R
by	RODRIGUEZ L.F. , ANGLADA G., CURIEL S.
	Astrophys. J., Suppl. Ser., 125, 427-438 (1999)
	The nature of the radio continuum sources embedded in the HH 7-11 region and its surroundings.
o	Tables 1, 2: <[RAC97] VLA NN> (Nos 5-44) added. Table 1, Fig.9: <[JCC87] IRAS 4C> added.
Ref:	=2000MNRAS.319..991S
by	SMITH K.W. , BONNELL I.A., EMERSON J.P., JENNESS T.
	Mon. Not. R. Astron. Soc., 319, 991-1000 (2000)
	NGC 1333/IRAS 4: a multiple star formation laboratory.
o	Components [JCC87] IRAS 4BI and 4BII are [JCC87] IRAS 4B1 and 4B2 in SIMBAD.
o	<[JCC87] IRAS ANA> (Nos 4B1, 4B2) added.
Ref:	=2001ApJ...546L..49S
by	SANDELL G. , KNEE L.B.G.
	Astrophys. J., 546, 49-52 (2001)
	NGC 1333–Protostars, dust shells, and triggered star formation.
o	Table 1: Components [JCC87] IRAS 4BW and 4BE are respectively [JCC87] IRAS 4B1 and 4B2 in SIMBAD.
o	Table 1: <[SK2001] NN> (Nos 1-33), <[SK2001] IRAS 7 SM N> (Nos 1-2). Table 1: <[JCC87] IRAS AN> (No. 2C) added.
=E=	Catalogue in electronic form as J/ApJS/125/427
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCF2004]
[JCF2004]	(Jordan+Cote+Ferrarese+, 2004)
Write:	<<[JCF2004] NNN>>
N:	174
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra ACIS observations of M 87.
in source:	M 87 = NGC 4486 = Virgo A
Ref:	=2004ApJ...613..279J
by	JORDAN A. , COTE P., FERRARESE L., BLAKESLEE J.P., MEI S., MERRITT D., MILOSAVLJEVIC M., PENG E.W., TONRY J.L., WEST M.J.
	Astrophys. J., 613, 279-301 (2004)
	The ACS Virgo cluster survey. III. Chandra and Hubble space telescope observations of low-mass X-ray binaries and globular clusters in M87.
o	Table 1: <[JCF2004] NNN> (Nos 1-174).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCF2006]
[JCF2006]	(Jorgensen+Chiboucas+Flint+, 2006) (Not yet in Simbad)
Write:	<<[JCF2006] J1226.9+3332 NNNN>>
N:	3
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Galaxies, members of the cluster RX J1226.9+3332.
in source:	RX J1226.0+3332
Ref:	=2006ApJ...639L...9J
by	JORGENSEN I. , CHIBOUCAS K., FLINT K., BERGMANN M., BARR J., DAVIES R.
	Astrophys. J., 639, 9-12 (2006)
	The fundamental plane for z = 0.8-0.9 cluster galaxies.
o	(Erratum) erratum vol. 654, p. L179 (2007)
o	Fig.1: <[JCF2006] J1226.9+3332 NNN> (Nos 711, 966).
Ref:	=2006ApJ...647L..99D
by	DI SEREGO ALIGHIERI S. , LANZONI B., JORGENSEN I.
	Astrophys. J., 647, 99-102 (2006)
	The influence of mass and environment on the evolution of early-type galaxies.
o	(Erratum) erratum vol. 652, p. L145 (2006)
o	RX J1226.9-3332 is a misprint for RX J1226.9+3332
o	Text: <[JCF2006] J1226.9+3332 NNN> (No. 563).
Ref:	=2009ApJS..184..271C
by	CHIBOUCAS K. , BARR J., FLINT K., JORGENSEN I., COLLOBERT M., DAVIES R.
	Astrophys. J., Suppl. Ser., 184, 271-287 (2009)
	The Gemini/HST cluster project: structural and photometric properties of galaxies in three z = 0.28-0.89 clusters.
o	Table 4: <[JCF2006] J1226.9+3332 NNN> N=112 among (Nos 18-1254).
o	Table 1: RX J0152.7+1357 is a misprint for RX J0152.7-1357.
=E=	Catalogue in electronic form as J/ApJS/184/271
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCF89]
[JCF89]	(Jacoby+Ciardullo+Ford+, 1989)
Write:	<<[JCF89] NNN>> <<[JCF89] a>>
N:	185+10
Object:	PN + * (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=185 PN in M 81. Table 2: N=10 standard stars (Nos a-j) in M 81. See also: Ford, [CJF89], [JCF90], [CJH91], [MCJ93], [JCH96], [FCJ97], [CJF98]
in source:	M 81 = NGC 3031
Ref:	=1989ApJ...344..704J
by	JACOBY G.H. , CIARDULLO R., FORD H.C., BOOTH J.
	Astrophys. J., 344, 704-714 (1989)
	Planetary nebulae as standard candles. III. The distance to M 81.
o	Tables 1, objects not in SIMBAD
o	Table 1: <[JCF89] NNN> (Nos 1-185). Table 2: <[JCF89] a> (Nos a-j).
=E=	Catalogue in electronic form as J/ApJ/344/704
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCF90]
[JCF90]	(Jacoby+Ciardullo+Ford, 1990)
Write:	<<[JCF90] NGC NNNN NNN>> <<[JCF90] NGC NNNN a>>
N:	810
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Format 'NNN' for PNs, format 'a' for reference stars. 1998ApJ...492...62C: Table 1: 'NGC 4486 NNN', N=339, numbering is following the numbering in the 1st ref. See also: Ford, [JCF89], [CJF89], [CJH91], [MCJ93], [JCH96], [FCJ97], [CJF98]
in source:	NGC 4374 = M 84
in source:	NGC 4382
in source:	NGC 4406 = M 86
in source:	NGC 4472 = M 49
in source:	NGC 4486 = M 87 = Virgo A
in source:	NGC 4649
Ref:	=1990ApJ...356..332J
by	JACOBY G.H. , CIARDULLO R., FORD H.C.
	Astrophys. J., 356, 332-349 (1990)
	Planetary nebulae as standard candles. V. The distance to the Virgo cluster.
o	Table 4: <[JCF90] NGC 4374 NNN> (Nos 1-102). Table 5: [JCF90] NGC 4382 NNN> (Nos 1-102). Table 6: <[JCF90] NGC 4406 NNN> (Nos 1-141). Table 7: <[JCF90] NGC 4472 NN> (Nos 1-54). Table 8: <[JCF90] NGC 4486 NN> (Nos 1-55). Table 9: <[JCF90] NGC 4649 NN> (Nos 1-32). Table 10: <[JCF90] NGC NNNN a> N=8+6+8+7+6+5.
Ref:	=1998ApJ...492...62C
by	CIARDULLO R. , JACOBY G.H., FELDMEIER J.J., BARTLETT R.E.
	Astrophys. J., 492, 62-73 (1998)
	The planetary nebula luminosity function of M 87 and the intracluster stars of Virgo.
o	in NGC 4486, 10 PN from 1990ApJ...356..332J ([JCF90] NGC 4486) not found in this study.
o	Table 1: <[JCF90] NGC 4486 NNN> (Nos 56-339) added. Table 2: <[CJF98] NGC 4478 N> (Nos 1-7), <[CJF98] IC 3443 N> No. 1, <[CJF98] Anon N> No. 1.
=E=	Catalogue in electronic form as J/ApJ/356/332
=E=	Catalogue in electronic form as J/ApJ/492/62
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCG2019]
[JCG2019]	(Jacobs+Collett+Glazebrook+, 2019)= ([JCG2019a])
Write:	<<[JCG2019] DES JHHMM+DDMM>>
N:	84
Object:	Poss. Grav. lens (SIMBAD class: GravLens_Candidate = Gravitational Lens Candidate)
Note:	N=84 gravitational lens candidates in the Dark Energy survey (DES) Year 3 imaging data. See also [JCG2019b].
Ref:	=2019MNRAS.484.5330J
by	JACOBS C. , COLLETT T., GLAZEBROOK K., McCARTHY C., QIN A.K., ABBOTT T.M.C., ABDALLA F.B., ANNIS J., AVILA S., BECHTOL K., BERTIN E., BROOKS D., BUCKLEY-GEER E., BURKE D.L., CARNERO ROSELL A., CARRASCO KIND M., CARRETERO J., DA COSTA L.N., DAVIS C., DE VICENTE J., DESAI S., DIEHL H.T., DOEL P., EIFLER T.F., FLAUGHER B., FRIEMAN J., GARCIA-BELLIDO J., GAZTANAGA E., GERDES D.W., GOLDSTEIN D.A., GRUEN D., GRUENDL R.A., GSCHWEND J., GUTIERREZ G., HARTLEY W.G., HOLLOWOOD D.L., HONSCHEID K., HOYLE B., JAMES D.J., KUEHN K., KUROPATKIN N., LAHAV O., LI T.S., LIMA M., LIN H., MAIA M.A.G., MARTINI P., MILLER C.J., MIQUEL R., NORD B., PLAZAS A.A., SANCHEZ E., SCARPINE V., SCHUBNELL M., SERRANO S., SEVILLA-NOARBE I., SMITH M., SOARES-SANTOS M., SOBREIRA F., SUCHYTA E., SWANSON M.E.C., TARLE G., VIKRAM V., WALKER A.R., ZHANG Y., ZUNTZ J., (The DES Collaboration)
	Mon. Not. R. Astron. Soc., 484, 5330-5349 (2019)
	Finding high-redshift strong lenses in DES using convolutional neural networks.
o	Figs 10-12, Table 4: <[JCG2019] DES JHHMM+DDMM> N=84.
=E=	Catalogue in electronic form as <J/MNRAS/484/5330/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCG2019a]
[JCG2019a]	(Jacobs+Collett+Glazebrook+, 2019)
*****	Avoid the usage of [JCG2019a], prefer [JCG2019]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCG2019b]
[JCG2019b]	(Jacobs+Collett+Glazebrook+, 2019) (Not yet in Simbad)
Write:	<<[JCG2019b] DES JHHMM+DDMM>>
N:	511
Object:	Poss. Grav. lens (SIMBAD class: GravLens_Candidate = Gravitational Lens Candidate)
Note:	N=511 gravitational lens candidates in the Dark Energy survey (DES) Year 3 imaging data. See also [JCG2019].
Ref:	=2019ApJS..243...17J
by	JACOBS C. , COLLETT T., GLAZEBROOK K., BUCKLEY-GEER E., DIEHL H.T., LIN H., McCARTHY C., QIN A.K., ODDEN C., CASO ESCUDERO M., DIAL P., YUNG V.J., GAITSCH S., PELLICO A., LINDGREN K.A., ABBOTT T.M.C., ANNIS J., AVILA S., BROOKS D., BURKE D.L., CARNERO ROSELL A., CARRASCO KIND M., CARRETERO J., DA COSTA L.N., DE VICENTE J., FOSALBA P., FRIEMAN J., GARCIA-BELLIDO J., GAZTANAGA E., GOLDSTEIN D.A., GRUEN D., GRUENDL R.A., GSCHWEND J., HOLLOWOOD D.L., HONSCHEID K., HOYLE B., JAMES D.J., KRAUSE E., KUROPATKIN N., LAHAV O., LIMA M., MAIA M.A.G., MARSHALL J.L., MIQUEL R., PLAZAS A.A., ROODMAN A., SANCHEZ E., SCARPINE V., SERRANO S., SEVILLA-NOARBE I., SMITH M., SOBREIRA F., SUCHYTA E., SWANSON M.E.C., TARLE G., VIKRAM V., WALKER A.R., ZHANG Y., (The DES Collaboration)
	Astrophys. J., Suppl. Ser., 243, 17-17 (2019)
	An extended catalog of galaxy-galaxy strong gravitational lenses discovered in DES using convolutional neural networks.
o	Fig. 4, Table 1: <[JCG2019b] DES JHHMM+DDMM> N=511.
=E=	Catalogue in electronic form as <J/ApJS/243/17/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCH96]
[JCH96]	(Jacoby+Ciardullo+Harris, 1996)
Write:	<<[JCH96] NGC NNNN NNN>> <<[JCH96] NGC NNNN a>> <<[JCH96] NGC NNNN OSN>>
N:	39+183+35+46+10
Object:	PN + * (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	Table 2: PN in NGC 4278, format 'NGC 4278 NN', (Nos 1-39). Table 3: PN in NGC 4494, format 'NGC 4494 NNN', (Nos 1-183). Table 4: PN in NGC 4565, format 'NGC 4565 NN', (Nos 1-35). Table 6: reference stars in NGC 4278, format 'NGC 4278 a, (Nos a-k). reference stars in NGC 4494, format 'NGC 4494 a, (Nos a-l). reference stars in NGC 4565, format 'NGC 4565 a, (Nos a-w). Table 10: Overluminous Source ('OS' in the format): in NGC 4278, (Nos OS1-OS2). in NGC 4382: (No. OS1). in NGC 4406: (Nos OS1-OS3). in NGC 4374: (Nos OS1-OS3). in NGC 4486: (No. OS1) See also: Ford, [JCF89], [CJF89], [JCF90], [CJH91], [MCJ93], [FCJ97], [CJF98]
in source:	NGC 4278
in source:	NGC 4494
in source:	NGC 4565
Ref:	=1996ApJ...462....1J
by	JACOBY G.H. , CIARDULLO R., HARRIS W.E.
	Astrophys. J., 462, 1-12 (1996)
	Planetary nebulae as standard candles. X. Tests in the Coma I region.
o	Table 2: <[JCH96] NGC 4278 NN> (Nos 1-39). Table 3: <[JCH96] NGC 4494 NNN> (Nos 1-183). Table 4: <[JCH96] NGC 4565 NN> (Nos 1-35). Table 6: <[JCH96] NGC NNNN a> N=46. Table 10: <[JCH96] NGC NNNN OSN> N=10. Certains objets n'ont pas de coordonnees.
=E=	Catalogue in electronic form as J/ApJ/462/1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCJ2014]
[JCJ2014]	(Juarez+Cargile+James+, 2014)
Write:	<<[JCJ2014] NNNNNa>>
N:	30
Object:	* (SIMBAD class: Star)
Note:	Gemini North GMOS observations of N=4+26 stars in the open Cluster Blanco 1.
in source:	Cl Blanco 1
Ref:	=2014ApJ...795..143J
by	JUAREZ A.J. , CARGILE P.A., JAMES D.J., STASSUN K.G.
	Astrophys. J., 795, 143 (2014)
	An improved determination of the lithium depletion boundary age of Blanco 1 and a first look on the effects of magnetic activity.
o	Tables 1+3: <[JCJ2014] NNNNNa> N=4+26 among (Nos 222-18237).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCL2014]
[JCL2014]	(Jauzac+Clement+Limousin+, 2014)
Write:	<<[JCL2014] NN>> <<[JCL2014] NN.N>>
N:	68+194
Object:	G + Grav. lensed image of a G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat.	in SIMBAD: Images (format NN.N) of Table 1 are completely incorporated)
Note:	HST ACS and WFC3 observations of N=194 images of N=68 multiply imaged galaxies gravitationally lensed by the cluster MCS J0416.1-2403.
in source:	MCS J0416.0-2403
Ref:	=2014MNRAS.443.1549J
by	JAUZAC M. , CLEMENT B., LIMOUSIN M., RICHARD J., JULLO E., EBELING H., ATEK H., KNEIB J.-P., KNOWLES K., NATARAJAN P., ECKERT D., EGAMI E., MASSEY R., REXROTH M.
	Mon. Not. R. Astron. Soc., 443, 1549-1554 (2014)
	Hubble Frontier Fields: a high-precision strong-lensing analysis of galaxy cluster MACSJ0416.1-2403 using ~ 200 multiple images.
o	Fig. 1, Table 2: <[JCL2014] NN> N=68 among (Nos 1-73), <[JCL2014] NN.N> N=194 among (Nos 1.1-1.3 to 73.1-73.2).
=E=	Catalogue in electronic form as <J/MNRAS/443/1549/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCL74]
[JCL74]	(Jones+Chetin+Liller, 1974)
Write:	<<[JCL74] Star A>>
N:	2
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	UHURU observations. Star E is poss. counterpart of LMC X-1. Star H is poss. counterpart of LMC X-3
Ref:	=1974ApJ...190L...1J
by	JONES C.A. , CHETIN T., LILLER W.
	Astrophys. J., 190, 1-3 (1974)
	Optical studies of UHURU sources. VIII. Observations of 92 possible counterparts of X-ray sources.
o	Table 1: GX 5-1 3 and 4 = [KOS70] GX 5-1 3 and 4. * V14 in NGC 6624 not identified
o	<[JCL74] Star E>, <[JCL74] Star H>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCM2013]
[JCM2013]	(Johnson+Chen+Maulchaey, 2013)
Write:	<<[JCM2013] NNNNN>>
N:	24+18
Object:	? + ALS (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Magellan telescopes IMACS and LDSS3 spectroscopy of the PKS 0405-123 field for a galaxy survey and a search for absorption line systems. Use of HST COS (UV) spectra.
Ref:	=2013MNRAS.434.1765J
by	JOHNSON S.D. , CHEN H.-W., MULCHAEY J.S.
	Mon. Not. R. Astron. Soc., 434, 1765-1778 (2013)
	Probing the IGM-galaxy connection at z > 0.5 - II. New insights into the galaxy environments of OVI absorbers in PKS 0405-123.
o	Table 2: <[JCM2013] NNNNN> N=24 among (Nos 80001-93242). Tables 3-6: <[JCM2013] PKS 0405-123 abs N.NNNNN> N=7+11.
=E=	Catalogue in electronic form as <J/MNRAS/434/1765/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCM2015]
[JCM2015]	(Johnson+Chen+Mulchaey, 2015)
Write:	<<[JCM2015] JHHMMSS.ss+DDMMSS.s>>
N:	148
Object:	G (SIMBAD class: Galaxy)
Note:	Magellan 6.5m telescope IMACS and LDSS3 spectroscopic observations of N=148 galaxies in the fields of HE 0226-4110, PKS 0405-123, LBQS 1435-0134, and PG 1522+101. Use of archival SDSS DR10 data.
Ref:	=2015MNRAS.449.3263J
by	JOHNSON S.D. , CHEN H.-W., MULCHAEY J.S.
	Mon. Not. R. Astron. Soc., 449, 3263-3273 (2015)
	On the possible environmental effect in distributing heavy elements beyond individual gaseous haloes.
o	Table 1: <[JCM2015] JHHMMSS.ss+DDMMSS.s> N=148.
=E=	Catalogue in electronic form as J/MNRAS/449/3263
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCM2017]
[JCM2017]	(Johnson+Chen+Mulchaey+, 2017)
Write:	<<[JCM2017] DNN>>
N:	18
Object:	Dwarf G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST COS spectroscopy of N=18 star-forming field dwarf galaxies. Use of Magellan telescopes spectroscopy.
Ref:	=2017ApJ...850L..10J
by	JOHNSON S.D. , CHEN H.-W., MULCHAEY J.S., SCHAYE J., STRAKA L.A.
	Astrophys. J., 850L, 10-10 (2017)
	The extent of chemically enriched gas around star-forming dwarf galaxies.
o	Table 1: <[JCM2017] DNN> (Nos D1-D18).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JCMT
JCMT	(James Clerk Maxwell Telescope) (Not yet in Simbad)
Write:	<<JCMT JHHMMSS.s+DDMMSS>>
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	Sources found using any of the JCMT instruments in survey mode. This includes searches through archival data. See also JCMTLSC, JCMTLSGC, JCMTLSJC, JCMTLSY, JCMTSF, JCMTSE.
Auth.:	CHRYSOSTOMOU A.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: JCMT
JCMT	(Matthews+McPhee+Fissel+, 2009)
*****	Avoid the usage of JCMT, prefer [MMF2009]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: JCMTLSC
JCMTLSC	(JCMT Legacy Survey. Cosmology Legacy Survey) (Not yet in Simbad)
Write:	<<JCMTLSC JHHMMSS.s+DDMMSS>>
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	In preparation. Sources found by the Cosmology Legacy Survey as part of the JCMT Legacy Survey project.
Auth.:	CHRYSOSTOMOU A.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: JCMTLSG
JCMTLSG	(JCMT Legacy Survey: Gould Belt Survey)
Write:	<<JCMTLSG JHHMMSS.s+DDMMSS>>
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	Sources found by the Gould Belt Survey as part of the JCMT Legacy Survey project.
Auth.:	CHRYSOSTOMOU A.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: JCMTLSP
JCMTLSP	(JCMT Legacy Survey: JCMT galactic Plane survey)
Write:	<<JCMTLSP JHHMMSS.s+DDMMSS>>
N:	7813
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	Sources found by the JCMT galactic Plane survey as part of the JCMT Legacy Survey project. 2017MNRAS.469.2163E: JCMT Plane Survey (JPS) Public Release 1 (N=7813 sources).
Ref:	=2017MNRAS.469.2163E
by	EDEN D.J. , MOORE T.J.T., PLUME R., URQUHART J.S., THOMPSON M.A., PARSONS H., DEMPSEY J.T., RIGBY A.J., MORGAN L.K., THOMAS H.S., BERRY D., BUCKLE J., BRUNT C.M., BUTNER H.M., CARRETERO D., CHRYSOSTOMOU A., CURRIE M.J., DEVILLIERS H.M., FICH M., GIBB A.G., HOARE M.G., JENNESS T., MANSER G., MOTTRAM J.C., NATARIO C., OLGUIN F., PERETTO N., PESTALOZZI M., POLYCHRONI D., REDMAN R.O., SALJI C., SUMMERS L.J., TAHANI K., TRAFICANTE A., DIFRANCESCO J., EVANS A., FULLER G.A., JOHNSTONE D., JONCAS G., LONGMORE S.N., MARTIN P.G., RICHER J.S., WEFERLING B., WHITE G.J., ZHU M.
	Mon. Not. R. Astron. Soc., 469, 2163-2183 (2017)
	The JCMT Plane Survey: first complete data release - emission maps and compact source catalogue.
o	Table 2, col. 1: <JPS GLLL.lll+BB.bbb> N=7813 = Table 2, col. 2: <JCMTLSP JHHMMSS.s+DDMMSS> N=7813.
=E=	Catalogue in electronic form as <J/MNRAS/469/2163/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: JCMTLSY
JCMTLSY	(JCMT Legacy Survey: SCUBA-2 All-Sky Survey)
Write:	<<JCMTLSY JHHMMSS.s+DDMMSS>>
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	Sources found by the SCUBA-2 All-Sky Survey as part of the JCMT Legacy Survey project.
Auth.:	CHRYSOSTOMOU A.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: JCMTPP
JCMTPP	(JCMT Public Legacy: Peak)
Write:	<<JCMTPP JHHMMSS.s+DDMMSS>>
Object:	Radio(sub-mm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	Public Legacy reductions of all JCMT SCUBA-2 (and ACSIS) will result in catalogues of peaks and extent. Peak catalogue acronym defined here. See also JCMTPX. More information is available on the JCMT Legacy Release 1 web page: https://www.eaobservatory.org/jcmt/science/archive/lr1/
Auth.:	Doug Johnstone d.johnstone@jach.hawaii.edu Joint Astronomy Centre
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: JCMTPX
JCMTPX	(JCMT Public Legacy: Extent)
Write:	<<JCMTPX JHHMMSS.s+DDMMSS>>
Object:	Radio(sub-mm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	Public Legacy reductions of all JCMT SCUBA-2 (and ACSIS) will result in catalogues of peaks and extent. Extent catalogue acronym defined here. See also JCMTPP. More information is available on the JCMT Legacy Release 1 web page: https://www.eaobservatory.org/jcmt/science/archive/lr1/
Auth.:	Doug Johnstone d.johnstone@jach.hawaii.edu Joint Astronomy Centre
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: JCMTSE
JCMTSE	(JCMT SCUBA Survey, Extended)
Write:	<<JCMTSE JHHMMSS.s+DDMMSS>>
N:	6118
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	JCMT SCUBA observations. This designation is intended for the Extended version of the catalogue. Extended Map Data Set: data regardless of the quality of the opacity calibration.
Ref:	=2008ApJS..175..277D
by	DI FRANCESCO J. , JOHNSTONE D., KIRK H., MacKENZIE T., LEDWOSINSKA E.
	Astrophys. J., Suppl. Ser., 175, 277-295 (2008)
	The SCUBA legacy catalogues: submillimeter-continuum objects detected by SCUBA.
o	Table 2: <JCMTSF JHHMMSS.s+DDMMSS> N=5061. Table 3: <JCMTSE JHHMMSS.s+DDMMSS> N=6118.
=E=	Catalogue in electronic form as J/ApJS/175/277
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: JCMTSF
JCMTSF	(JCMT Survey, SCUBA Fundamental)
Write:	<<JCMTSF JHHMMSS.s+DDMMSS>>
N:	5061
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	JCMT SCUBA observations. This designation is intended or the most secure (Fundamental) detections in the catalogue. Fundamental Map Data Set: data with superior opacity calibration.
Ref:	=2008ApJS..175..277D
by	DI FRANCESCO J. , JOHNSTONE D., KIRK H., MacKENZIE T., LEDWOSINSKA E.
	Astrophys. J., Suppl. Ser., 175, 277-295 (2008)
	The SCUBA legacy catalogues: submillimeter-continuum objects detected by SCUBA.
o	Table 2: <JCMTSF JHHMMSS.s+DDMMSS> N=5061. Table 3: <JCMTSE JHHMMSS.s+DDMMSS> N=6118.
=E=	Catalogue in electronic form as J/ApJS/175/277
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: JCO
JCO	(James-Cargile Optical (optical targets in the James, D. and Cargile P. catalogue)) (Not yet in Simbad)
Write:	<<JCO NNNN>>
N:	∼2500
Object:	* in Cl* (SIMBAD class: Star)
Note:	We have recently completed an optical survey (in UBVI filters), covering almost 2 square degrees, in and around the young open cluster Blanco 1. Using the CTIO 1m telescope, we have uniformly measured UBVI photometry for stars in the magnitude range, 10 < V < 17, which essentially encompasses all of the G, K and early M-stars in the cluster. We have already published some small excerpts of the photometric dataset in: Mermilliod et al. (2008A&A...485...95M), Cargile, James & Platais (2009AJ....137.3230C), Stauffer et al. (2010ApJ...719.1859S), Cargile, James & Jeffries (2010ApJ...725L.111C). We are currently writing an MNRAS paper to publish the entire photometric catalogue for all stars in the survey area, including newly acquired radial velocities. We will cross-correlate all photometrically identified cluster members with our already published X-rays, proper motions and higher-mass (brighter) work. We seek an acronym which will allow us to catalogue our stars in and around Blanco 1, putting them onto a coherent, uniform numbering system. Two further publications, in addition to the UBVI master paper, are scheduled to be written and will include differential photometry (for rotation periods) and Lithium spectra (for abundance determinations) that we have already obtained. http://astro.phy.vanderbilt.edu/~cargilpa/SPOCS/
in source:	Cl Blanco 1
Auth.:	David James CTIO djj@ctio.noao.edu
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [JCO2011]
[JCO2011]	(Jones+Crocker+Ott+, 2011)
Write:	<<[JCO2011] Sgr B2(AAA)>> <<[JCO2011] Sgr B2(AA)>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA observations at 1384 and 2368MHz of the Sagittarius B giant molecular cloud. See also [BJ84].
in source:	NAME SGR B:NAME SGR B1 = NAME SGR B1
in source:	NAME SGR B:NAME SGR B2 = NAME SGR B2
Ref:	=2011AJ....141...82J
by	JONES D.I. , CROCKER R.M., OTT J., PROTHEROE R.J., EKERS R.D.
	Astron. J., 141, 82 (2011)
	Australia telescope compact array radio continuum 1384 and 2368 MHz observations of Sagittarius B.
o	Fig. 1, Table 2: <[JCO2011] Sgr B2(AAA)> (Nos BBL, SC, ABC).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCR2013]
[JCR2013]	(Jablonka+Combes+Rines+, 2013)
Write:	<<[JCR2013] GALHHMM+DDMMA>> <<[JCR2013] GALHHMM+DDMM-A>> (not recognised by Simbad, but found in literature)
N:	3
Object:	IR luminous G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	IRAM PdBI observations of N=3 luminous infrared galaxies (LIRGs) inside the virial radii of two intermediate redshift clusters: CL1416+4446 (z=0.397) and CL0926+1242 (z=0.489). Use of archival Spitzer and HST data.
in source:	ClG J0926+1242
in source:	ClG J1416+4446
Ref:	=2013A&A...557A.103J
by	JABLONKA P. , COMBES F., RINES K., FINN R., WELCH T.
	Astron. Astrophys., 557A, 103-103 (2013)
	Cold gas in the inner regions of intermediate redshift clusters.
o	Table1: <[JCR2013] GALHHMM+DDMMA> (Nos GAL1416+4446, GAL0926+1242A, GAL0926+1242B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCS2018]
[JCS2018]	(Johnson+Chen+Straka+, 2018)
Write:	<<[JCS2018] GNN>> <<[JCS2018] PKS 0405-123 group>>
N:	30+1
Object:	Group of G + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	VLT MUSE observations of N=30 galaxies in the field of the quasar PKS 0405-123 quasar at z<1. Use of archival HST ACS images. See also [JCM2013].
Ref:	=2018ApJ...869L...1J
by	JOHNSON S.D. , CHEN H.-W., STRAKA L.A., SCHAYE J., CANTALUPO S., WENDT M., MUZAHID S., BOUCHE N., HERENZ E.C., KOLLATSCHNY W., MULCHAEY J.S., MARINO R.A., MASEDA M.V., WISOTZKI L.
	Astrophys. J., 869L, 1-1 (2018)
	Galaxy and quasar fueling caught in the act from the intragroup to the interstellar medium.
o	Table 1: <[JCS2018] GNN> (Nos G1-G30), <[JCS2018] PKS 0405-123 group> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCT2014]
[JCT2014]	(Jorgensen+Chiboucas+Toft+, 2014)
Write:	<<[JCT2014] NNNN>>
N:	54
Object:	G (SIMBAD class: Galaxy)
Note:	Gemini GMOS-N observations of N=54 galaxies in the field of the galaxy cluster RX J0848.6+4453. Use of HST ACS archival imaging.
in source:	RX J0848.6+4453
Ref:	=2014AJ....148..117J
by	JORGENSEN I. , CHIBOUCAS K., TOFT S., BERGMANN M., ZIRM A., SCHIAVON R.P., GRUTZBAUCH R.
	Astron. J., 148, 117 (2014)
	RX J0848.6+4453: the evolution of galaxy sizes and stellar populations in a z = 1.27 cluster.
o	Fig. 2, Table 10: <[JCT2014] NNNN> N=54 among (Nos 240-9001).
o	The good reference for Stott et al. 2010 is 2010ApJ...718...23S. RX J0848.6+4443, RX J0848.6+4445, RX J0848.6+4553 and RX J0848.9+4453 are probable misprints for RX J0848.6+4453.
=E=	Catalogue in electronic form as <J/AJ/148/117/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCW2004]
[JCW2004]	(Jordan+Cote+West+, 2004)
Write:	<<[JCW2004] NGC NNNN NNN>>
N:	207+322+359+124
Object:	Poss. GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of four galaxies: search for globular clusters.
in source:	NGC 541
in source:	NGC 2832
in source:	NGC 4839
in source:	NGC 7768
Ref:	=2004AJ....127...24J
by	JORDAN A. , COTE P., WEST M.J., MARZKE R.O., MINNITI D., REJKUBA M.
	Astron. J., 127, 24-47 (2004)
	Hubble space telescope observations of cD galaxies and their globular cluster systems.
o	Table 4: <[JCW2004] NGC 541 NNN> (Nos 1-207). Table 5: <[JCW2004] NGC 2832 NNN> (Nos 1-322). Table 6: <[JCW2004] NGC 4839 NNN> (Nos 1-359). Table 7: <[JCW2004] NGC 7768 NNN> (Nos 1-124).
=E=	Catalogue in electronic form as J/AJ/127/24
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCW2013]
[JCW2013]	(Jiang+Chen+Wang+, 2013) (Not yet in Simbad)
Write:	<<[JCW2013] ANa>>
N:	17
Object:	H2 feature (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=17 H2 jets and knots in the active star-forming region RAFGL 5157. USe of Spitzer/IRAC and SMA observations.
in source:	RAFGL 5157
Ref:	=2013RAA....13..695J
by	JIANG Z.-B. , CHEN Z.-W., WANG Y., YANG J., HUANG J.-S., ZHANG Q.-Z., FAZIO G.
	RAA, 13, 695-704 (2013)
	AFGL 5157 NH_{3}: a new stellar cluster in the forming process.
o	Fig. 2, Paragr. 3.1: <[JCW2013] ANa> (Nos R1, R1a-R1b, R2-R3, B1, B1a-B1b, B2-B3, J1-J4, Y1-Y3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JCW2018]
[JCW2018]	(Jorgensen+Chiboucas+Webb+, 2018)
Write:	<<[JCW2018] ANNNN NNNN>>
N:	149+169
Object:	G (SIMBAD class: Galaxy)
Note:	Gemini GMOS-N observations of N=149+169 galaxies in the galaxy clusters ACO 2029 and ACO 2142 respectively. Use of SDSS DR14 and DR7 data.
in source:	ACO 2029
in source:	ACO 2142
Ref:	=2018AJ....156..224J
by	JORGENSEN I. , CHIBOUCAS K., WEBB K., WOODRUM C.
	Astron. J., 156, 224-224 (2018)
	The Gemini/Hubble Space Telescope Galaxy Cluster Project: stellar populations in the low-redshift reference cluster galaxies.
o	Tables 14-16: <[JCW2018] ANNNN NNNN> N=149+169 among (Nos A2029 9-A2029 6346, A2142 4-A2142 8368).
=E=	Catalogue in electronic form as <J/AJ/156/224/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JD
JD	(J-band Dropout)
*****	Avoid the usage of JD, prefer [HMC2008]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [JD2002]
[JD2002]	(Jacoby+De Marco, 2002)
Write:	<<[JD2002] NN>> <<[JD2002] JHHMMSS.s+DDMMSS.s>>
N:	25+1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	N=25 new PNs in the SMC, (Nos 1-25), and N=1 PN candidate 'J005719.7-721314.5'.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2002AJ....123..269J
by	JACOBY G.H. , DE MARCO O.
	Astron. J., 123, 269-278 (2002)
	A survey for very faint planetary nebulae in the SMC. I. Identification, confirmation, and preliminary analysis.
o	Table 3: <[JD2002] NN> (Nos 1-25). Text: <[JD2002] JHHMMSS.s+DDMMSS.s> N=1. T.4 : LHA 115-N 9, 61 et 68 : coord fournies par Brian Skiff (CathB sept2002)
=E=	Catalogue in electronic form as J/AJ/123/269
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JD2012]
[JD2012]	(Jones+Dickey, 2012)
Write:	<<[JD2012] GLLL.lll+BB.bbb>>
N:	185
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	N=185 HII regions. Use of radio and infrared archival data from the VLA Galactic Plane Survey (VGPS), Southern Galactic Plane Survey (SGPS), WISE, GLIMPSE.
Ref:	=2012ApJ...753...62J
by	JONES C. , DICKEY J.M.
	Astrophys. J., 753, 62 (2012)
	Kinematic distance assignments with H I absorption.
o	Table 2: <[JD2012] GLLL.lll+BB.bbb> N=185.
=E=	Catalogue in electronic form as J/ApJ/753/62
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JDC2021]
[JDC2021]	(Jones+De Gasperin+Cuciti+, 2021)
Write:	<<[JDC2021] PSZ2 G096.88+24.18 W Relic>> <<[JDC2021] PSZ2 G096.88+24.18 S Relic W>>
N:	2+2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	LOFAR High Band Antenna (HBA) 140MHz and VLA 1.5GHz observations of N=2 relics in PSZ2 G096.88+24.18 and and N=2 shocks in the southern relic.
in source:	PSZ2 G096.88+24.18
Ref:	=2021MNRAS.505.4762J
by	JONES A. , DE GASPERIN F., CUCITI V., HOANG D.N., BOTTEON A., BRUGGEN M., BRUNETTI G., FINNER K., FORMAN W.R., JONES C., KRAFT R.P., SHIMWELL T., VAN WEEREN R.J.
	Mon. Not. R. Astron. Soc., 505, 4762-4774 (2021)
	Radio relics in PSZ2 G096.88+24.18: a connection with pre-existing plasma.
o	Fig. 5, Table 3: <[JDC2021] PSZ2 G096.88+24.18 W Relic> (Nos N, S), <[JDC2021] PSZ2 G096.88+24.18 S Relic W> (Nos E, W).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JDG98]
[JDG98]	(Johnson+De Pree+Goss, 1998)
Write:	<<[JDG98] N>>
N:	4
Object:	H2O Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	HST HRS observations. Table 9: N=4 H2O masers (Nos 1-4), in M 17. Nos 1 and 2 have already been studied in 1977A&AS...30..145G
in source:	M 17 = NGC 6618
Ref:	=1998ApJ...500..302J
by	JOHNSON C.O. , DEPREE C.G., GOSS W.M.
	Astrophys. J., 500, 302-310 (1998)
	A high-resolution VLA study of M17-UC1.
o	UC 1 = [FCM84] M17 UC-1.
o	Table 9: <[JDG98] N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JDH94]
[JDH94]	(Jarrett+Dickman+Herbst, 1994)
Write:	<<[JDH94] Tau NNNN>> <<[JDH94] Oph NNN>>
N:	31+16
Object:	* (SIMBAD class: Star)
Note:	Tables 1, 2, 4: 12+8+11 Taurus foreground candidates, format 'Tau NNNN'. Tables 3, 5: 11+5 Ophiuchus foreground candidates, format 'Oph NNN'.
Ref:	=1994ApJ...424..852J
by	JARRETT T.H. , DICKMAN R.L., HERBST W.
	Astrophys. J., 424, 852-869 (1994)
	An optical study of the faint end of the stellar luminosity function.
o	T. 1,2,4: <[JDH94] Tau NNNN> N=31. T. 3,5: <[JDH94] Oph NNN> N=16
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JDJ2006]
[JDJ2006]	(Jones+Drinkwater+Jurek+, 2006)= (UCD) = (VUCD)
Write:	<<[JDJ2006] N>>
N:	9
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	2dF multifiber spectrograph on the Anglo-Australian telescope observations: search for Ultracompact dwarf (UCD) galaxies in the Virgo Cluster. See also VCO for the coordinates format.
in source:	NAME Virgo Cluster
Ref:	=2006AJ....131..312J
by	JONES J.B. , DRINKWATER M.J., JUREK R., PHILLIPPS S., GREGG M.D., BEKKI K., COUCH W.J., KARICK A., PARKER Q.A., SMITH R.M.
	Astron. J., 131, 312-324 (2006)
	Discovery of ultracompact dwarf galaxies in the Virgo cluster.
o	Table 2: <[JDJ2006] N> (Nos 1-9) = <VCO JHHMMSS.s+DDMMSS> N=9.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JDP2019]
[JDP2019]	(Jayasinghe+Dixon+Povich+, 2019)= (MWP) = (MWP2)
Write:	<<[JDP2019] MWP2GLLLllll+BBbbbbb>>
N:	2600+599
Object:	(IR) + Bubble + Bowshock (SIMBAD class: Infrared = Infra-Red Source)
Stat.	in SIMBAD: Table 3 entrée
Note:	The second data release (DR2) for the Milky Way Project (MWP), which includes an updated catalogue of N=2600 IR bubbles identified by the collective work of >31 000 citizen scientists visually inspecting survey images from the GLIMPSE, MIPSGAL, SMOG, and Cygnus-X surveys of the Galactic plane. MWPDR2 also includes the first citizen-science catalogue of N=599 IR bowshock driving star candidates (BDSCs), including 311 newly discovered objects. See also [SPK2012] for the first data release. More information is available on the online citizen science website 'The Milky Way Project': http://www.milkywayproject.org
Ref:	=2019MNRAS.488.1141J
by	JAYASINGHE T. , DIXON D., POVICH M.S., BINDER B., VELASCO J., LEPORE D.M., XU D., OFFNER S., KOBULNICKY H.A., ANDERSON L.D., KENDREW S., SIMPSON R.J.
	Mon. Not. R. Astron. Soc., 488, 1141-1165 (2019)
	The Milky Way Project second data release: bubbles and bow shocks.
o	Tables 3+6: <[JDP2019] MWP2GLLLllll+BBbbbbb> N=2600+599.
=E=	Catalogue in electronic form as <J/MNRAS/488/1141/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JDW2009]
[JDW2009]	(Johnson+Dong+Wang, 2009)
Write:	<<[JDW2009] GLLL.lll+B.bbb>> <<[JDW2009] GLLL.lll+B.bb>> <<[JDW2009] GLLL.ll+B.bbb>> <<[JDW2009] GLLL.ll+B.bb>>
N:	17
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Identification of X-ray filaments in Chandra ACIS observations of the Galactic Center.
in source:	NAME Galactic Center
Ref:	=2009MNRAS.399.1429J
by	JOHNSON S.P. , DONG H., WANG Q.D.
	Mon. Not. R. Astron. Soc., 399, 1429-1440 (2009)
	A large-scale survey of X-ray filaments in the galactic centre.
o	Tables 1-2: <[JDW2009] GLLL.lll+B.bbb>, <[JDW2009] GLLL.lll+B.bb>, <[JDW2009] GLLL.ll+B.bbb>, <[JDW2009] GLLL.ll+B.bb> N=17.
Details on Acronym: [JE82]
[JE82]	(Jaschek+Egret, 1982)
Write:	<<[JE82] NNNN>>
N:	1159
Object:	Be* (SIMBAD class: Star)
Note:	Catalog of Be stars, found re-numbered 'NNNN' in literature.
Ref:	=1982IAUS...98..261J
by	JASCHEK M. , EGRET D.
	IAU Symp. 98, held in Munich, Federal Republic of Germany, April 6-10, 1981.Ed. M. Jaschek and H.-G. Groth. " Be Stars"., 98, 261-None (1982)
	A catalogue of Be stars.
o	<[JE82] NNNN> N=1147 among (Nos 1-1159).
=E=	Catalogue in electronic form as III/67
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JEG
JEG	(J.E. Geach)
*****	Avoid the usage of JEG, prefer [GSR2007]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [JEG2005]
[JEG2005]	(Jones+Edge+Grainge+, 2005)
Write:	<<[JEG2005] ACO NNNN +xxx+yyy>>
N:	4+9+6
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	15 GHz radio observations of X-ray clusters with the Ryle Telescope, with images from ROSAT and ASCA. In the format '+xxx+yyy' stands for offsets from the radio pointing centres.
in source:	ACO 697
in source:	ACO 1914
in source:	ACO 2218
Ref:	=2005MNRAS.357..518J
by	JONES M.E. , EDGE A.C., GRAINGE K., GRAINGER W.F., KNEISSL R., POOLEY G.G., SAUNDERS R., MIYOSHI S.J., TSURUTA T., YAMASHITA K., TAWARA Y., FURUZAWA A., HARADA A., HATSUKADE I.
	Mon. Not. R. Astron. Soc., 357, 518-526 (2005)
	H_0 from an orientation-unbiased sample of Sunyaev-Zel'dovich and X-ray clusters.
o	In table 1 : Z2701 = ZwCl 2701, RXJ1720 = RX J1720.0+2637.
o	Table 3: <[JEG2005] ACO NNNN +xxx+yyy> N=4+9+6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JEK2011]
[JEK2011]	(Jiang+Egami+Kashikawa+, 2011)
Write:	<<[JEK2011] NN>>
N:	19
Object:	LBG (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Keck DEIMOS observations of N=19 z>6 Lyman break galaxies in the Subaru Deep Field.
in source:	NAME SDF
Ref:	=2011ApJ...743...65J
by	JIANG L. , EGAMI E., KASHIKAWA N., WALTH G., MATSUDA Y., SHIMASAKU K., NAGAO T., OTA K., OUCHI M.
	Astrophys. J., 743, 65 (2011)
	Keck spectroscopy of lyman-break galaxies and its implications for the UV-continuum and Lyα luminosity functions at z > 6.
o	Figs 1-2, Table 1: <[JEK2011] NN> (Nos 1-19).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JEM2013]
[JEM2013]	(Jiang+Egami+Mechtley+, 2013)
Write:	<<[JEM2013] NN>>
N:	67
Object:	G (SIMBAD class: Galaxy)
Note:	Deep HST NIR and Spitzer MIR observations of N=67 spectroscopically confirmed galaxies at z≥6, in the Subaru Deep Field (SDF) and the Subaru XMM-Newton Deep Survey (SXDS) field.
in source:	NAME SDF
in source:	NAME SXDSF
Ref:	=2013ApJ...772...99J
by	JIANG L. , EGAMI E., MECHTLEY M., FAN X., COHEN S.H., WINDHORST R.A., DAVE R., FINLATOR K., KASHIKAWA N., OUCHI M., SHIMASAKU K.
	Astrophys. J., 772, 99 (2013)
	Physical properties of spectroscopically confirmed galaxies at z ≥ 6. I. Basic characteristics of the rest-frame UV continuum and Lyα emission.
o	Fig. 12, Tables 1-2: <[JEM2013] NN> (Nos 1-67).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Jena
Jena	(Jena univ.)
Write:	<<Jena NN>> <<Jena A>>
N:	37+5
Object:	Extr. Red * (SIMBAD class: Infrared = Infra-Red Source)
Note:	(Nos 1-37), Identif. charts. Obj. 28, 31, 32 are found to be spurious in the 2nd ref. (Nos A-E), Jena A = Jena 17, Jena B = Jena 18
Ref:	=1973AN....294..153D
by	DORSCHNER J. , FRIEDEMANN C., GURTLER J.
	Astron. Nachr., 294, 153-158 (1973)
	A search for extremely red stars on the Palomar Observatory sky survey.
o	Table 1: <Jena NN> (Nos 1-37)
Ref:	=1977AN....298..327F
by	FRIEDEMANN C. , GURTLER J., PFAU W.
	Astron. Nachr., 298, 327-329 (1977)
	A search for extremely red stars, on the Palomar Observatory sky survey. II. Examination for light variability.
o	Table I: <Jena A> (Nos A-E)
Details on Acronym: Jenkins
Jenkins	(Jenkins)
====>	Equivalent to: PLX
Details on Acronym: [JEP2006]
[JEP2006]	(Jeffries+Evans+Pye+, 2006)= (SAS)
Write:	<<[JEP2006] NNN>>
N:	163
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton observations of NGC 2547.
in source:	NGC 2547
Ref:	=2006MNRAS.367..781J
by	JEFFRIES R.D. , EVANS P.A., PYE J.P., BRIGGS K.R.
	Mon. Not. R. Astron. Soc., 367, 781-800 (2006)
	An XMM-Newton observation of the young open cluster NGC 2547: coronal activity at 30 Myr.
o	Tables 1, 3: <[JEP2006] NNN> (Nos 1-163).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JES2016]
[JES2016]	(Jauzac+Eckert+Schwinn+, 2016)
Write:	<<[JES2016] Core>> <<[JES2016] N>> <<[JES2016] NW>> <<[JES2016] Wbis>> <<[JES2016] SN>>
N:	1+1+1+1+4
Object:	Grav. lensed image of a G (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy)
Stat.	in SIMBAD: Table 4 is not in Simbad.
Note:	HST ACS observations of N=1+1+1+1+4 substructures in the field of the Hubble Frontier Fields cluster Abell 2744. Application of a strong and weak lensing model. Use of MPG/ESO 2.2m telescope WFI and CFHT archival data.
in source:	ACCG 118 = ACO 2744
Ref:	=2016MNRAS.463.3876J
by	JAUZAC M. , ECKERT D., SCHWINN J., HARVEY D., BAUGH C.M., ROBERTSON A., BOSE S., MASSEY R., OWERS M., EBELING H., SHAN H.Y., JULLO E., KNEIB J., RICHARD J., ATEK H., CLEMENT B., EGAMI E., ISRAEL H., KNOWLES K., LIMOUSIN M., NATARAJAN P., REXROTH M., TAYLOR P., TCHERNIN C.
	Mon. Not. R. Astron. Soc., 463, 3876-3893 (2016)
	The extraordinary amount of substructure in the Hubble Frontier Fields cluster Abell 2744.
o	Fig. 4, Table 2: <[JES2016] Core> N=1, <[JES2016] N> N=1, <[JES2016] NW> N=1, <[JES2016] Wbis> N=1, <[JES2016] SN> (Nos S1-S4). Fig. 4, Table 4: <[JES2016] XN> (Nos X1-X4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JES2018]
[JES2018]	(Jauzac+Eckert+Schaller+, 2018)
Write:	<<[JES2018] MACS J0717 Core>> <<[JES2018] MACS J0717 WWN>> <<[JES2018] MACS J0717 XNN>>
N:	1+9+10
Object:	Substructure + (X-ray) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=1+9 substructures and N=10 X-ray emitting cluster remnant cores in the field of the galaxy cluster MCS J0717.5+3745. Use of HST, Subaru, and CFHT imaging, of Chandra and XMM-Newton imaging, and of Keck-II, Keck-I, and Gemini-North spectroscopy.
in source:	ClG J0717+3745 = MCS J0717.5+3745
Ref:	=2018MNRAS.481.2901J
by	JAUZAC M. , ECKERT D., SCHALLER M., SCHWINN J., MASSEY R., BAHE Y., BAUGH C., BARNES D., DALLA VECCHIA C., EBELING H., HARVEY D., JULLO E., KAY S.T., KNEIB J.-P., LIMOUSIN M., MEDEZINSKI E., NATARAJAN P., NONINO M., ROBERTSON A., TAM S.I., UMETSU K.
	Mon. Not. R. Astron. Soc., 481, 2901-2917 (2018)
	Growing a 'cosmic beast': observations and simulations of MACS J0717.5+3745.
o	Fig. 2, Table 1: <[JES2018] MACS J0717 Core> N=1, <[JES2018] MACS J0717 WWN> (Nos SW1-SW2, SE1-SE5, NE1-NE2). Fig. 2, Table 2: <[JES2018] MACS J0717 XNN> (Nos X1-X10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Jessup
Jessup	(Discoverer's name)
*****	Avoid the usage of Jessup, prefer Jsp
Details on Acronym: [JFA2008]
[JFA2008]	(Jiang Fan+Annis+, 2008)
Write:	<<[JFA2008] JHHMMSS.ss+DDMMSS.s>>
N:	6
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	MMT SWIRC NIR and KeckII LRIS observations of N=6 high redshift QSOs.
Ref:	=2008AJ....135.1057J
by	JIANG L. , FAN X., ANNIS J., BECKER R.H., WHITE R.L., CHIU K., LIN H., LUPTON R.H., RICHARDS G.T., STRAUSS M.A., JESTER S., SCHNEIDER D.P.
	Astron. J., 135, 1057-1066 (2008)
	A survey of z ~ 6 quasars in the sloan digital sky survey deep stripe. I. A flux-limited sample at z_{AB}< 21.
o	Table 1: Except for the first object, the QSOs are not in the SDSS DR5 catalogue.
o	Table 1: <[JFA2008] JHHMMSS.ss+DDMMSS.s> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JFA99]
[JFA99]	(Jager+Fricke+Appenzeller+, 1999)
Write:	<<[JFA99] a>>
N:	20
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	FORS1 VLT observations. N=20 galaxies in the field of QSO 0307-0015.
Ref:	=1999A&A...352L..17J
by	JAEGER K. , FRICKE K.J., APPENZELLER I., SZEIFERT T., HEIDT J., GAESSLER W., HAEFNER R., HUMMEL W., MUSCHIELOK B., NICKLAS H., SEIFERT W., STAHL O.
	Astron. Astrophys., 352, 17-21 (1999)
	Imaging and spectroscopy with FORS1 in the field of Q 0307-0015.
o	Fig.1, Table 1: <[JFA99] a> (Nos a-t).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JFB2009]
[JFB2009]	(Jiang+Fan+Bian+, 2009)
Write:	<<[JFB2009] JHHMMSS.ss+DDMMSS.s>>
N:	6
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	KPNO SQIID and Magellan PANIC NIR photometry and MMT Red Channel Spectrograph optical spectroscopy of N=6 QSOs at z∼2. See also [JFA2008].
Ref:	=2009AJ....138..305J
by	JIANG L. , FAN X., BIAN F., ANNIS J., CHIU K., JESTER S., LIN H., LUPTON R.H., RICHARDS G.T., STRAUSS M.A., MALANUSHENKO V., MALANUSHENKO E., SCHNEIDER D.P.
	Astron. J., 138, 305-311 (2009)
	A survey of z ~ 6 quasars in the Sloan Digital Sky Survey deep stripe. II. Discovery of six quasars at z_{AB}>21.
o	Table 1: <[JFB2009] JHHMMSS.ss+DDMMSS.s> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JFC2010]
[JFC2010]	(Jackson+Finn+Chambers+, 2010)
Write:	<<[JFC2010] GLLL.ll+BB.bb>> <<[JFC2010] GLLL.l+BB.bb>>
N:	11+1
Object:	Dense Core (SIMBAD class: denseCore = Dense Core)
Stat:	is completely incorporated in Simbad
Note:	ATNF Mopra 22m telescope HCN(1-0) observations of N=12 compact, dense molecular cores in the Nessie Nebula.
in source:	NAME Nessie Nebula
Ref:	=2010ApJ...719L.185J
by	JACKSON J.M. , FINN S.C., CHAMBERS E.T., RATHBORNE J.M., SIMON R.
	Astrophys. J., 719L, 185-189 (2010)
	The "Nessie" nebula: cluster formation in a filamentary infrared dark cloud.
o	Table 1: <[JFC2010] GLLL.ll+BB.bb> N=11, <[JFC2010] GLLL.l+BB.bb> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JFH99]
[JFH99]	(Jorgensen+Franx+Hjorth+, 1999)
Write:	<<[JFH99] ACO 665 NNNN>> <<[JFH99] ACO 2218 NNNN>>
N:	37+1
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	HST WFPC2 observations of ACO 665 and ACO 2218.
in source:	ACO 665
in source:	ACO 2218
Ref:	=1999MNRAS.308..833J
by	JORGENSEN I. , FRANX M., HJORTH J., VAN DOKKUM P.G.
	Mon. Not. R. Astron. Soc., 308, 833-853 (1999)
	The evolution of cluster E and SO galaxies measured from the Fundamental Plane.
o	Table A2: in ACO 2218, LNNN = LPS NNN, BOWNNN = BOW ACO 2218 CCNNN.
o	Table A1: <[JFH99] ACO 665 NNNN> N=37 among (Nos 1022-2159). Table A2: <[JFH99] ACO 2218 NNNN> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JFK
JFK	(Jorgensen+Franx+Kjaergaard)
*****	Avoid the usage of JFK, prefer [JFK95]
Origin	of the Acronym: L (2001MNRAS.327..265H)
Details on Acronym: [JFK95]
[JFK95]	(Jorgensen+Franx+Kjaergaard, 1995)= (J) = (JFK)
Write:	<<[JFK95] ACO 194 NNN>> <<[JFK95] ACO S 639 NNN>>
N:	1+7
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Table 3: '[JFK95] ACO 194 101', N=1 galaxy in ACO 194, named ANON 101 by the authors. '[JFK95] ACO S 639 NNN', N=16 galaxies in ACO S 639 among (Nos 6-109)
Ref:	=1995MNRAS.273.1097J
by	JORGENSEN I. , FRANX M., KJAERGAARD P.
	Mon. Not. R. Astron. Soc., 273, 1097-1128 (1995)
	Multicolour CCD surface photometry for E and SO galaxies in 10 clusters.
o	ACO 3381 = DRCG 0608-33, so G in ACO 3381 are named '[D80] DRCG 0608-33 NNA'
o	Table 3: <[D80] DRCG 0608-33 NNA> (No. 34B), <[D80] DRCG 2345-28 NNN> (Nos 101-105), <[JFK95] ACO 194 NNN> (No. 101), <[JFK95] ACO S 639 NN> N=7 among (Nos 6-23)
Ref:	=1995MNRAS.276.1341J
by	JORGENSEN I. , FRANX M., KJAERGAARD P.
	Mon. Not. R. Astron. Soc., 276, 1341-1364 (1995)
	Spectroscopy for E and S0 galaxies in nine clusters.
o	Table 4: <[JFK95] ACO S 639 NNN> N=16 among (Nos 6-109), 9 are new
=E=	Catalogue in electronic form as J/MNRAS/273/1097
=E=	Catalogue in electronic form as <J/MNRAS/276/1341/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JFM2001]
[JFM2001]	(Johnstone+Fich+Mitchell+, 2001)= (SMM)
Write:	<<[JFM2001] SMM JHHMMmm+DDMMm>>
N:	75
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SCUBA observations. N=75 850mu.m clumps in Ori B (North). See also OriBsmm and Paper II: [JMM2006].
in source:	NAME Ori B
Ref:	=2001ApJ...559..307J
by	JOHNSTONE D. , FICH M., MITCHELL G.F., MORIARTY-SCHIEVEN G.
	Astrophys. J., 559, 307-317 (2001)
	Large area mapping at 850 microns. III. Analysis of the clump distribution in the Orion B molecular cloud.
o	Table 1: <[JFM2001] SMM JHHMMmm+DDMMm> N=75.
=E=	Catalogue in electronic form as J/ApJ/559/307
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JGB98]
[JGB98]	(Johansson+Greve+Booth+, 1998)
Write:	<<[JGB98] 30 Dor-NN>> <<[JGB98] N158-N>> <<[JGB98] N160-N>> <<[JGB98] N159-W>> <<[JGB98] N159-N>>
N:	33+5+6+3+3
Object:	CO Cloud (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	Table 1: CO Cloud in 30 Dor, N158, 159, 160 = LHA 120-N 158, 159, 160. See also [KRB97]
in source:	Magellanic Clouds:LMC:30 Dor Nebula = 30 Dor Nebula
in source:	Magellanic Clouds:LMC:LHA 120-N 158 = LHA 120-N 158
in source:	Magellanic Clouds:LMC:LHA 120-N 159 = LHA 120-N 159
in source:	Magellanic Clouds:LMC:LHA 120-N 160 = LHA 120-N 160
Ref:	=1998A&A...331..857J
by	JOHANSSON L.E.B. , GREVE A., BOOTH R.S., BOULANGER F., GARAY G., DE GRAAUW T., ISRAEL F.P., KUTNER M.L., LEQUEUX J., MURPHY D.C., NYMAN L.-A., RUBIO M.
	Astron. Astrophys., 331, 857-872 (1998)
	Results of the SEST key programme: CO in the Magellanic Clouds. VII. 30 Doradus and its southern H II regions.
o	Table 1: <[JGB98] 30 Dor-NN> (Nos 1-33), <[JGB98] N158-N> (Nos 1-5), <[JGB98] N160-N> (Nos 1-6), <[JGB98] N159-W> (Nos E, W, S), <[JGB98] N159-N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JGC2017]
[JGC2017]	(Jacobs+Glazebrook+Collett+, 2017) (Not yet in Simbad)
Write:	<<[JGC2017] CNNN>> <<[JGC2017] CNNN system>>
N:	16+16
Object:	Poss. Grav. lens + Poss. Grav. lens system (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=16+16 gravitational lens and system candidates, found in CFHTLS data by using convolutional neural networks (ConvNets, CN).
Ref:	=2017MNRAS.471..167J
by	JACOBS C. , GLAZEBROOK K., COLLETT T., MORE A., McCARTHY C.
	Mon. Not. R. Astron. Soc., 471, 167-181 (2017)
	Finding strong lenses in CFHTLS using convolutional neural networks.
o	Fig. 6, Table 6: <[JGC2017] CNNN> (Nos CN1-CN16), <[JGC2017] CNNN system> (Nos CN1 system-CN16 system).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JGC98]
[JGC98]	(Jha+Garnavich+Challis+, 1998)
Write:	<<[JGC98] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Galaxy near SN 1998DI (not a SN).
Ref:	=1998IAUC.6983Q...1J
by	JHA S. , GARNAVICH P., CHALLIS P., KIRSHNER R., BERLIND P.
	IAU Circ., 6983, 1-None (1998)
	1998di.
o	<[JGC98] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JGD81]
[JGD81]	(Jaffe+Gusten+Downes, 1981)
Write:	<<[JGD81] H2O LLL.ll+B.bb>> <<[JGD81] H2O LLL.lll+B.bbb>> <<[JGD81] FIR LLL.ll+B.bb>>
N:	26+20
Object:	Maser + (IR) (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	See also [JSF82]
Ref:	=1981ApJ...250..621J
by	JAFFE D.T. , GUSTEN R., DOWNES D.
	Astrophys. J., 250, 621-630 (1981)
	New H2O masers associated with far-infrared sources.
o	Table 1 col(1): <[JGD81] H2O LLL.ll+B.bb> or <[JGD81] H2O LLL.lll+B.bbb> N=26, associated with Table 1 col(5): <[JGD81] FIR LLL.ll+B.bb> N=20
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JGD88]
[JGD88]	(Jones+Garwood+Dickey, 1988)= (IR)
Write:	<<[JGD88] LL.lll>>
N:	33+41
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Table 1: N=33 IR candidates. Table 2: N=41 radio-sources without IR candidates
Ref:	=1988ApJ...328..559J
by	JONES T.J. , GARWOOD R., DICKEY J.M.
	Astrophys. J., 328, 559-568 (1988)
	Compact radio sources in the Galactic plane.
o	Tables 1, 2: <[JGD88] LL.lll> N=33+41
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JGF2013]
[JGF2013]	(JARDEL+GEBHARDT+FABRICIUS+, 2013)
Write:	<<[JGF2013] NN>>
N:	12
Object:	* (SIMBAD class: Star)
Note:	McDonald Observatory 2.7 m Harlan J. Smith telescope VIRUS-W spectroscopy of N=12 stars in the Draco dwarf galaxy.
in source:	NAME Draco Galaxy
Ref:	=2013ApJ...763...91J
by	JARDEL J.R. , GEBHARDT K., FABRICIUS M.H., DRORY N., WILLIAMS M.J.
	Astrophys. J., 763, 91 (2013)
	Measuring dark matter profiles non-parametrically in dwarf spheroidals: an application to Draco.
o	Table 1: <[JGF2013] NN> (Nos 1-12).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JGF93]
[JGF93]	(Jannuzi+Green, 1993)= (OP)
Write:	<<[JGF93] HHMM+DD>>
N:	2
Object:	QSO (SIMBAD class: QSO = Quasar)
Ref:	=1993ApJ...404..100J
by	JANNUZI B.T. , GREEN R.F., FRENCH H.
	Astrophys. J., 404, 100-111 (1993)
	An optical polarization survey for BL Lacertae objects and highly polarized quasars.
o	<[JGF93] 1106+36>, <[JGF93] 0229+06>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JGJ90]
[JGJ90]	(Johnson+Gehrz+Jones+, 1990)
Write:	<<[JGJ90] NN>>
N:	17
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	OMC:OMC 2 = OMC 2
Ref:	=1990AJ....100..518J
by	JOHNSON J.J. , GEHRZ R.D., JONES T.J., HACKWELL J.A., GRASDALEN G.L.
	Astron. J., 100, 518-529 (1990)
	An infrared study of Orion molecular cloud-2 (OMC-2).
o	Table II: <[JGJ90] NN> N=17
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JGK99]
[JGK99]	(Jha+Garnavich+Kirshner+, 1999)
Write:	<<[JGK99] N>>
N:	6
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=6 comparison stars in the field of SN 1998BU.
Ref:	=1999ApJS..125...73J
by	JHA S. , GARNAVICH P.M., KIRSHNER R.P., CHALLIS P., SODERBERG A.M., MACRI L.M., HUCHRA J.P., BARMBY P., BARTON E.J., BERLIND P., BROWN W.R., CALDWELL N., CALKINS M.L., KANNAPPAN S.J., KORANYI D.M., PAHRE M.A., RINES K.J., STANEK K.Z., STEFANIK R.P., SZENTGYORGYI A.H., VAISANEN P., WANG Z., ZAJAC J.M., RIESS A.G., FILIPPENKO A.V., LI W., MODJAZ M., TREFFERS R.R., HERGENROTHER C.W., GREBEL E.K., SEITZER P., JACOBY G.H., BENSON P.J., RIZVI A., MARSCHALL L.A., GOLDADER J.D., BEASLEY M., VACCA W.D., LEIBUNDGUT B., SPYROMILIO J., SCHMIDT B.P., WOOD P.R.
	Astrophys. J., Suppl. Ser., 125, 73-97 (1999)
	The type Ia supernova 1998bu in M96 and the Hubble constant.
o	Table 1, Fig.1: <[JGK99] N> (Nos 1-6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JGS92]
[JGS92]	(Johnston+Gaume+Stolovy+, 1992)
Write:	<<[JGS92] NNA>>
N:	17+7
Object:	CH3OH Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	Map in the 2 references
in source:	OMC:OMC 1 = OMC 1
Ref:	=1992ApJ...385..232J
by	JOHNSTON K.J. , GAUME R., STOLOVY S., WILSON T.L., WALMSLEY C.M., MENTEN K.M.
	Astrophys. J., 385, 232-239 (1992)
	The distribution of the 6 2-6 1 and 5 2-5 1 E-type methanol masers in OMC-1.
o	Tables 1, 2: <[JGS92] NN> (Nos 1-15)
Ref:	=1997ApJ...490..758J
by	JOHNSTON K.J. , GAUME R.A., WILSON T.L., NGUYEN H.A., NEDOLUHA G.E.
	Astrophys. J., 490, 758-764 (1997)
	The apparent sizes of the 6 2-6 1 E-type methanol masers in OMC-1.
o	Table 1: <[JGS92] NNA> (Nos 7A-7B, 9A-9B, 11A-11C, 16-17) added
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JGT99]
[JGT99]	(Johnson+Gilmore+Tanvir+, 1999) (Not yet in Simbad)
Write:	<<[JGT99] NN>>
N:	39
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
in source:	NAME HST'S
Ref:	=1999NewA....4..431J
by	JOHNSON R.A. , GILMORE G.F., TANVIR N.R., ELSON R.A.W.
	New Astronomy, 4, 431-441 (1999)
	A survey of unresolved objects in the Hubble Deep Field South.
o	Table 2: <[JGT99] NN> (Nos 1-39).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JH
JH	(Jones+Herbig)
Write:	<<JH NNN>>
N:	245
Object:	* (SIMBAD class: Star)
Note:	Table III: (Nos 1-237) and (Nos 426-433)
Ref:	=1979AJ.....84.1872J
by	JONES B.F. , HERBIG G.H.
	Astron. J., 84, 1872-1889 (1979)
	Proper motions of T Tauri variables and other stars associated with the Taurus-Auriga dark clouds.
o	<JH NNN> N=245 (Nos 1-237 and 426-433)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: JH
JH	(Janes+Hoq)
====>	Equivalent to: [JH2011]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: JH
JH	(Jones+Hyland)
*****	Avoid the usage of JH, prefer [JH80]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [JH2011]
[JH2011]	(Janes+Hoq, 2011)= (JH)
Write:	<<[JH2011] Be NN NNNNN>> <<[JH2011] King NN NNNN>> <<[JH2011] NGC NNNN NNNNN>>
N:	24351+13684+30187
Object:	* (SIMBAD class: Star)
Note:	Perkins telescope PRISM observations of N=68222 stars in the field of distant open clusters.
in source:	Cl Berkeley 19
in source:	Cl Berkeley 44
in source:	Cl King 25
in source:	NGC 6802
in source:	NGC 6827
in source:	Cl Berkeley 52
in source:	Cl Berkeley 56
in source:	NGC 7142
in source:	NGC 7245
in source:	Cl King 9
Ref:	=2011AJ....141...92J
by	JANES K.A. , HOQ S.
	Astron. J., 141, 92 (2011)
	A quantitative analysis of distant open clusters.
o	Table 9: <[JH2011] Be NN NNNNN> N=24351, <[JH2011] King NN NNNN> N=13684, <[JH2011] NGC NNNN NNNNN> N=30187.
=E=	Catalogue in electronic form as J/AJ/141/92
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JH80]
[JH80]	(Jones+Hyland, 1980)= (JH)
Write:	<<[JH80] N>>
N:	9
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1980MNRAS.192..359J
by	JONES T.J. , HYLAND A.R.
	Mon. Not. R. Astron. Soc., 192, 359-364 (1980)
	New results on interstellar reddening in the near infrared.
o	<[JH80] N> N=9
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JH97]
[JH97]	(Jaunsen+Hjorth, 1997)
Write:	<<[JH97] B1600+434>> <<[JH97] B1600+434 Lens>> <<[JH97] B1600+434 A>> <<[JH97] B1600+434 SE>> <<[JH97] Star N>>
N:	1+1+2+1+4
Object:	G + * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Image of the gravitational lens CLASS B1600+434 = [JH97] B1600+434: 1 lens 'B1600+434 Lens'. 2 lensing images [JH97] B1600+434 A and B. 1 galaxy named here 'SE'. In the field of the lens: 4 stars (Nos 1-4). See also [KDJ98] and [FC98].
Ref:	=1997A&A...317L..39J
by	JAUNSEN A.O. , HJORTH J.
	Astron. Astrophys., 317, 39-None (1997)
	Detection of a spiral lens galaxy and optical variability in the gravitational lens system B1600+434.
o	Table 3: <[JH97] B1600+434> N=1, <[JH97] B1600+434 Lens> N=1, <[JH97] B1600+434 A> (Nos A-B), <[JH97] B1600+434 SE>. Fig 1: <[JH97] Star N> (Nos 1-3).
Ref:	=2000ApJ...544..117B
by	BURUD I. , HJORTH J., JAUNSEN A.O., ANDERSEN M.I., KORHONEN H., CLASEN J.W., PELT J., PIJPERS F.P., MAGAIN P., OSTENSEN R.
	Astrophys. J., 544, 117-122 (2000)
	An optical time delay estimate for the double gravitational lens system B1600+434.
o	Fig.2: <[JH97] Star N> (No. 4) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JHA98]
[JHA98]	(Jaunsen+Hjorth+Andersen+, 1998)
Write:	<<[JHA98] Star A>>
N:	13
Object:	* (SIMBAD class: Star)
Note:	N=13 comparison stars in the field of GRB 980519.
Ref:	=1998GCN....78....1J
by	JAUNSEN A.O. , HJORTH J., ANDERSEN M.I., KJERNSMO K., PEDERSEN H., PALAZZI E.
	GRB Coordinates Network, Circular Service, 78, 1-None (1998)
	GRB980519 optical observations.
o	<[JHA98] Star A> (Nos A-D).
Ref:	=1998GCN....87....1B
by	BLOOM J.S. , DJORGOVSKI S.G., GAL R.R., KULKARNI S.R., KELLY A.
	GRB Coordinates Network, Circular Service, 87, 1-None (1998)
	GRB 980519 optical observations.
o	<[JHA98] Star A> (Nos G-L, K missing).
Ref:	=2001ApJ...546..127J
by	JAUNSEN A.O. , HJORTH J., BJORNSSON G., ANDERSEN M.I., PEDERSEN H., KJERNSMO K., KORHONEN H., SORENSEN P.M., PALAZZI E.
	Astrophys. J., 546, 127-133 (2001)
	The jet and circumburst stellar wind of GRB 980519.
o	Table 1: <[JHA98] Star A> (Nos M-N).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JHC
JHC	(Jacoby+Hunter+Christian)
*****	Avoid the usage of JHC, prefer [JHC84]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JHC2008]
[JHC2008]	(Johnston-Hollitt+Hunstead+Corbett, 2008)
Write:	<<[JHC2008] NNN>>
N:	143
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	AAT 2dF observations of ACO 3667.
in source:	ACO 3667
Ref:	=2008A&A...479....1J
by	JOHNSTON-HOLLITT M. , HUNSTEAD R.W., CORBETT E.
	Astron. Astrophys., 479, 1-8 (2008)
	The optical morphology of A3667 re-examined.
o	Table 2: <[JHC2008] NNN> (Nos 1-143).
=E=	Catalogue in electronic form as J/A+A/479/1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JHC82]
[JHC82]	(Jones+Hyland+Caswell+, 1982)
Write:	<<[JHC82] LLL.l+B.b>> <<[JHC82] LLL.ll+B.bb>>
N:	49
Object:	OH/IR (SIMBAD class: Infrared = Infra-Red Source)
Ref:	=1982ApJ...253..208J
by	JONES T.J. , HYLAND A.R., CASWELL J.L., GATLEY I.
	Astrophys. J., 253, 208-223 (1982)
	A search for the infrared counterpart of type II OH masers. II. Statistical analysis.
o	<[JHC82] LLL.ll+B.bb> N=49.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JHC84]
[JHC84]	(Jacoby+Hunter+Christian, 1984)= (JHC)
Write:	<<[JHC84] NNN>>
N:	161
Object:	O-M * (SIMBAD class: Star)
Ref:	=1984ApJS...56..257J
by	JACOBY G.H. , HUNTER D.A., CHRISTIAN C.A.
	Astrophys. J., Suppl. Ser., 56, 257-281 (1984)
	A library of stellar spectra.
o	<[JHC84] NNN> (Nos 1-161).
=E=	Catalogue in electronic form as III/92
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JHE2006]
[JHE2006]	(Jorgensen+Harvey+Evans II+, 2006)
Write:	<<[JHE2006] L1448-C(W)>> <<[JHE2006] JHHMMSS+DDMMSS>>
N:	2+4
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Spitzer Space Telescope IR camera (IRAC) observations of LDN 1448 and LDN 1455: N=2 sources in the outflow of LDN 1448, and 2 knots in each LDN.
in source:	LDN 1448
in source:	LDN 1455
Ref:	=2006ApJ...645.1246J
by	JORGENSEN J.K. , HARVEY P.M., EVANS II N.J., HUARD T.L., ALLEN L.E., PORRAS A., BLAKE G.A., BOURKE T.L., CHAPMAN N., CIEZA L., KOERNER D.W., LAI S.-P., MUNDY L.G., MYERS P.C., PADGETT D.L., REBULL L., SARGENT A.I., SPIESMAN W., STAPELFELDT K.R., VAN DISHOECK E.F., WAHHAJ Z., YOUNG K.E.
	Astrophys. J., 645, 1246-1263 (2006)
	The Spitzer c2d survey of large, nearby, interstellar clouds. III. Perseus observed with IRAC.
o	Fig.14: <[BC86b] LDN 1455 IRS N> (Nos 4-6) added. Table 5: <[JHE2006] L1448-C(W)> (Nos C(N), C(S)). Paragr. 6.1, 6.2: <[JHE2006] JHHMMSS+DDMMSS> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JHF2003]
[JHF2003]	(Jakobsson+Hjorth+Fynbo+, 2003)
Write:	<<[JHF2003] A>>
N:	8
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=8 secondary calibration stars in the field of GRB 011211.
Ref:	=2003A&A...408..941J
by	JAKOBSSON P. , HJORTH J., FYNBO J.P.U., GOROSABEL J., PEDERSEN K., BURUD I., LEVAN A., KOUVELIOTOU C., TANVIR N., FRUCHTER A., RHOADS J., GRAV T., HANSEN M.W., MICHELSEN R., ANDERSEN M.I., JENSEN B.L., PEDERSEN H., THOMSEN B., WEIDINGER M., BHARGAVI S.G., COWSIK R., PANDEY S.B.
	Astron. Astrophys., 408, 941-947 (2003)
	The afterglow and the host galaxy of GRB 011211.
o	Table 2: <[JHF2003] A> (Nos A-H).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JHF2004]
[JHF2004]	(Jakobsson+Hjorth+Fynbo+, 2004)
Write:	<<[JHF2004] JHHMM.m+DDMM.m>>
N:	1
Object:	Absorber
Note:	A galaxy 'J1213.1-2054.8' is seen at 1".2 of GRB 030429 optical afterglow. See also [WFH2003].
Ref:	=2004A&A...427..785J
by	JAKOBSSON P. , HJORTH J., FYNBO J.P.U., WEIDINGER M., GOROSABEL J., LEDOUX C., WATSON D., BJOERNSSON G., GUDMUNDSSON E.H., WIJERS R.A.M.J., MOLLER P., PEDERSEN K., SOLLERMAN J., HENDEN A.A., JENSEN B.L., GILMORE A., KILMARTIN P., LEVAN A., CASTRO CERON J.M., CASTRO-TIRADO A.J., FRUCHTER A., KOUVELIOTOU C., MASETTI N., TANVIR N.
	Astron. Astrophys., 427, 785-794 (2004)
	The line-of-sight towards GRB 030429 at z=2.66: Probing the matter at stellar, galactic and intergalactic scales.
o	Table 2: <[JHF2004] JHHMM.m+DDMM.m> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JHK2002]
[JHK2002]	(Jayawardhana+Holland+Kalas+, 2002)
Write:	<<[JHK2002] N>>
N:	3
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	SCUBA and HST NICMOS observations. N=3 smm sources toward 55 Cnc system.
Ref:	=2002ApJ...570L..93J
by	JAYAWARDHANA R. , HOLLAND W.S., KALAS P., GREAVES J.S., DENT W.R.F., WYATT M.C., MARCY G.W.
	Astrophys. J., 570, 93-96 (2002)
	New submillimeter limits on dust in the 55 Cancri planetary system.
o	Table 1: <[JHK2002] N> (Nos 1-3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JHK2012]
[JHK2012]	(Jaeger+Hyman+Kassim+, 2012)
Write:	<<[JHK2012] JHHMMSS.s+DDMMSS>>
N:	8+2
Object:	Variable Radio Source + Transient (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 325MHz observations of N=8 variable sources and N=1 transient source in the SWIRE deep field 1046+59.
Ref:	=2012AJ....143...96J
by	JAEGER T.R. , HYMAN S.D., KASSIM N.E., LAZIO T.J.W.
	Astron. J., 143, 96 (2012)
	Discovery of a meter-wavelength radio transient in the SWIRE deep field: 1046+59.
o	Table 2, Text: <[JHK2012] JHHMMSS.s+DDMMSS> N=8+2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JHO2019]
[JHO2019]	(Jorgensen+Hunter+O'Neill+, 2019)
Write:	<<[JHO2019] NNNN>>
N:	82
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	HST ACS and Gemini North GMOS-N observations of N=82 galaxies in the galaxy clusters Lynx E and Lynx W. See also [JCT2014].
in source:	Lynx supercluster:Lynx E = Lynx E
in source:	Lynx supercluster:Lynx W = Lynx W
Ref:	=2019ApJ...881...42J
by	JORGENSEN I. , HUNTER L.C., O'NEILL C.R., CHIBOUCAS K., COLE R.K., TOFT S., SCHIAVON R.P.
	Astrophys. J., 881, 42-42 (2019)
	The Gemini/HST galaxy cluster project: environment effects on the stellar populations in the Lynx clusters at z = 1.27.
o	Table 7: <[JHO2019] NNNN> N=82 among (Nos 104-5037).
=E=	Catalogue in electronic form as <J/ApJ/881/42/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JHR80]
[JHR80]	(Jones+Hyland+Robinson+, 1980)= (Csk)
Write:	<<[JHR80] A-NNa>>
N:	75+27+10
Object:	* (SIMBAD class: Star)
Note:	The map is divided into 3 blocks D, E, and F. In block D: (Nos D-1 to D-38, D-41 to D-72, 6a, 7a, 15a and 15b). In block E: (Nos E-1 to E-27). In block F: N=10 among (Nos F-4 and F-23).
in source:	Tapia 2
Ref:	=1980ApJ...242..132J
by	JONES T.J. , HYLAND A.R., ROBINSON G., SMITH R., THOMAS J.
	Astrophys. J., 242, 132-140 (1980)
	Infrared observations of a Bok globule in the southern Coalsack.
o	Table 1: <[JHR80] D-NNa> N=43, <[JHR80] E-NN> N=27, <[JHR80] F-NNa> N=10
Ref:	=1984ApJ...282..675J
by	JONES T.J. , HYLAND A.R., BAILEY J.
	Astrophys. J., 282, 675-682 (1984)
	The inner core of a Bok globule.
o	Table 1: <[JHR80] D-NN> N=32 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JHS2010]
[JHS2010]	(Johansson+Horellou+Sommer+, 2010)
Write:	<<[JHS2010] NN>>
N:	17
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	APEX LABOCA 870mum observations of the Bullet cluster.
in source:	ClG 0657-56
Ref:	=2010A&A...514A..77J
by	JOHANSSON D. , HORELLOU C., SOMMER M.W., BASU K., BERTOLDI F., BIRKINSHAW M., LANCASTER K., LOPEZ-CRUZ O., QUINTANA H.
	Astron. Astrophys., 514A, 77-77 (2010)
	Submillimeter galaxies behind the Bullet cluster (1E 0657-56).
o	Table 2: <[JHS2010] NN> (Nos 1-17).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JHS2017]
[JHS2017]	(Jose+Herczeg+Samal+, 2017)
Write:	<<[JHS2017] DDD.dddd+DD.dddd>>
N:	1326
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	UH 2.2m telescope observations of N=1326 sources in Cl Stock 8. Use of archival UKIDSS DR6 and Spitzer IRAC warm mission.
in source:	Cl Stock 8
Ref:	=2017ApJ...836...98J
by	JOSE J. , HERCZEG G.J., SAMAL M.R., FANG Q., PANWAR N.
	Astrophys. J., 836, 98-98 (2017)
	The low-mass population in the young cluster Stock 8: stellar properties and initial mass function.
o	Table 2: <[JHS2017] DDD.dddd+DD.dddd> N=1326.
=E=	Catalogue in electronic form as <J/ApJ/836/98/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JHS86]
[JHS86]	(Jones+Hyland+Straw+, 1986)
Write:	<<[JHS86] N10-Na>> <<[JHS86] N59A-N>> <<[JHS86] N158C-N>> <<[JHS86] N160A-N>> <<[JHS86] N160C-N>> <<[JHS86] N159-NN>> <<[JHS86] N159 PN>>
N:	29+68+2
Object:	* (SIMBAD class: Star)
Note:	Table 2(a): * in the field of: N10 = LHA 120-N 10, (Nos 1, 2a-2b, 3-7). N59A = LHA 120-N 59A, (Nos 1-4). N158C = LHA 120-N 158C, (Nos 1-4). N160A = LHA 120-N 160A, (Nos 1-9). N160C = LHA 120-N 160C, (Nos 1-4). Table 2(b): * in the field of: N159 = LHA 120-N 159, (Nos 1-68), + 2 protostars (Nos P1-P2). Map in Fig.2. See also Paper II: [GHJ82]
in source:	Magellanic Clouds:LMC:LHA 120-N 10 = LHA 120-N 10
in source:	Magellanic Clouds:LMC:LHA 120-N 59A = LHA 120-N 59A
in source:	Magellanic Clouds:LMC:LHA 120-N 158C = LHA 120-N 158C
in source:	Magellanic Clouds:LMC:LHA 120-N 160A = LHA 120-N 160A
in source:	Magellanic Clouds:LMC:LHA 120-N 159 = LHA 120-N 159
Ref:	=1986MNRAS.219..603J
by	JONES T.J. , HYLAND A.R., STRAW S., HARVEY P.M., WILKING B.A., JOY M., GATLEY I., THOMAS J.A.
	Mon. Not. R. Astron. Soc., 219, 603-627 (1986)
	Star formation in the Magellanic clouds - III. IR observations of giant HII regions.
o	cross-id. CCH = [CCH78] LMC X-1 NN, [GHJ82] LMC N159 KN, [DD75] LMC X-1 NN.
o	Table 2(a): <[JHS86] N10-Na> (Nos 1, 2a-2b, 3-7), <[JHS86] N59A-N> (Nos 1-4), <[JHS86] N158C-N> (Nos 1-4), <[JHS86] N160A-N> (Nos 1-9), <[JHS86] N160C-N> (Nos 1-4). Table 2(b): <[JHS86] N159-NN> (Nos 1-68), <[JHS86] N159 PN> (Nos P1-P2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JI
JI	(J. Irwin)
*****	Avoid the usage of JI, prefer UMJI
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [JII2010]
[JII2010]	(Jeon+Im+Ibrahimov+, 2010)
Write:	<<[JII2010] WNN NNNNN>>
N:	117815
Object:	(Opt) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Maidanak Observatory 1.5-m telescope BRI observations of N=117815 sources in the field of the AKARI North Ecliptic Pole Wide Survey.
in source:	NAME NEP
Ref:	=2010ApJS..190..166J
by	JEON Y. , IM M., IBRAHIMOV M., LEE H.M., LEE I., LEE M.G.
	Astrophys. J., Suppl. Ser., 190, 166-180 (2010)
	Optical images and source catalog of AKARI North Ecliptic Pole wide survey field.
o	Table 4: <[JII2010] WNN NNNNN> N=117815.
=E=	Catalogue in electronic form as J/ApJS/190/166
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JIK2014]
[JIK2014]	(Jeon+Im+Kang+, 2014)
Write:	<<[JIK2014] FF NNNNN>> <<[JIK2014] FLMFF_NNNNN>> (not recognised by Simbad, but found in literature)
N:	295383
Object:	(NIR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	KPNO FLAMINGOS NIR observations of N=295383 sources in the AKARI North Ecliptic Pole field.
in source:	NAME NEP
Ref:	=2014ApJS..214...20J
by	JEON Y. , IM M., KANG E., LEE H.M., MATSUHARA H.
	Astrophys. J., Suppl. Ser., 214, 20 (2014)
	J- and H-band imaging of AKARI North Ecliptic Pole survey field.
o	Table 6: <[JIK2014] FF NNNNN> N=295383.
=E=	Catalogue in electronic form as J/ApJS/214/20
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JINGLE
JINGLE	(JCMT dust and gas In Nearby Galaxies Legacy Exploration)
Write:	<<JINGLE NNN>>
N:	193
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	JCMT SCUBA-2 850µm observations of N=193 galaxies in the local universe. Use of MaNGA and SDSS DR14 data.
Ref:	=2018MNRAS.481.3497S
by	SAINTONGE A. , WILSON C.D., XIAO T., LIN L., HWANG H.S., TOSAKI T., BUREAU M., CIGAN P.J., CLARK C.J.R., CLEMENTS D.L., DE LOOZE I., DHARMAWARDENA T., GAO Y., GEAR W.K., GREENSLADE J., LAMPERTI I., LEE J.C., LI C., MICHALOWSKI M.J., MOK A., PAN H.-A., SANSOM A.E., SARGENT M., SMITH M.W.L., WILLIAMS T., YANG C., ZHU M., ACCURSO G., BARMBY P., BRINKS E., BOURNE N., BROWN T., CHUNG A., CHUNG E.J., CIBINEL A., COPPIN K., DAVIES J., DAVIS T.A., EALES S., FANCIULLO L., FANG T., GAO Y., GLASS D.H.W., GOMEZ H.L., GREVE T., HE J., HO L.C., HUANG F., JEONG H., JIANG X., JIAO Q., KEMPER F., KIM J.H., KIM M., KIM T., KO J., KONG X., LACAILLE K., LACEY C.G., LEE B., LEE J.H., LEE W.-K., MASTERS K., OH S.-H., PAPADOPOULOS P., PARK C., PARK S.-J., PARSONS H., ROWLANDS K., SCICLUNA P., SCUDDER J.M., SETHURAM R., SERJEANT S., SHAO Y., SHEEN Y.-K., SHI Y., SHIM H., SMITH C.M.A., SPEKKENS K., TSAI A.-L., VERMA A., URQUHART S., VIOLINO G., VITI S., WAKE D., WANG J., WOUTERLOOT J., YANG Y., YIM K., YUAN F., ZHENG Z.
	Mon. Not. R. Astron. Soc., 481, 3497-3519 (2018)
	JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies - I. Survey overview and first results.
o	Table 2: <JINGLE NNN> (Nos 0-192).
=E=	Catalogue in electronic form as <J/MNRAS/481/3497/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [JIP2003]
[JIP2003]	(Johnson+Indebetouw+Pisano, 2003)
Write:	<<[JIP2003] IC 4662-W>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Radio data of IC 4662, using the Australia Telescope Compact Array, is compared to optical data from the HST archives. N=2 radio peaks East and North of [HMM90] A1 region. See also [HMM90].
in source:	IC 4662
Ref:	=2003AJ....126..101J
by	JOHNSON K.E. , INDEBETOUW R., PISANO D.J.
	Astron. J., 126, 101-112 (2003)
	Searching for embedded super-star clusters in IC 4662, NGC 1705, and NGC 5398.
o	Fig.1, Table 3: <[JIP2003] IC 4662-W> (Nos E, N).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JIW2004]
[JIW2004]	(Johnson+Indebetouw+Watson, 2004)
Write:	<<[JIW2004] AN>>
N:	3
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA observations of [H56] 3 (Haro 3). The region [SSM96] A contains 3 radio-sources A1 to A3.
in source:	[H56] 3 = Mrk 35 = NGC 3353
Ref:	=2004AJ....128..610J
by	JOHNSON K.E. , INDEBETOUW R., WATSON C., KOBULNICKY H.A.
	Astron. J., 128, 610-616 (2004)
	Revealing the young starburst in Haro 3 with radio and infrared imaging.
o	Fig.1b, Table 2: <[JIW2004] AN> (Nos A1-A3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JJ
JJ	(Jones+Jones)= (G)
Write:	<<JJ NNNA>>
N:	92 among 159
Object:	G in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
in source:	NAME Fornax Cluster
Ref:	=1980MNRAS.191..685J
by	JONES J.E. , JONES B.J.T.
	Mon. Not. R. Astron. Soc., 191, 685-700 (1980)
	The Fornax cluster of galaxies.
o	format JJ 119' not in SIMBAD
o	Table 1: <JJ NNNA> N=92 among (Nos 1-159)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [JJ97]
[JJ97]	(Jorgensen+Jimenez, 1997)
Write:	<<[JJ97] Cluster 1 NN>> <<[JJ97] Cluster 3 NN>>
N:	51+30
Object:	* in Cl* (SIMBAD class: Star)
Note:	Table 1: * in Cluster 1, N=51 among (Nos 2-68). Table 2: * in Cluster 3, N=30 among (Nos 1-34). Finding charts in Figs 1, 2
in source:	NAME Fornax 1
in source:	NAME Fornax 3
Ref:	=1997A&A...317...54J
by	JORGENSEN U.G. , JIMENEZ R.
	Astron. Astrophys., 317, 54-64 (1997)
	Globular clusters 1 and 3 in the Fornax dwarf galaxy.
o	Table 1: <[JJ97] Cluster 1 NN> N=51 among (Nos 2-68). Table 2: <[JJ97] Cluster 3 NN> N=30 among (Nos 1-34)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JJE2015]
[JJE2015]	(Jauzac+Jullo+Eckert+, 2015)
Write:	<<[JJE2015] AN>>
N:	6
Object:	Grav. lens + (X) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=2 dark matter haloes (CN), N=2 substructures (SN), and N=2 X-ray peaks (XN) in the field of the galaxy cluster MCS J0416.1-2403. Use of HST and Chandra data.
in source:	MCS J0416.1-2403
Ref:	=2015MNRAS.446.4132J
by	JAUZAC M. , JULLO E., ECKERT D., EBELING H., RICHARD J., LIMOUSIN M., ATEK H., KNEIB J.-P., CLEMENT B., EGAMI E., HARVEY D., KNOWLES K., MASSEY R., NATARAJAN P., NEICHEL B., REXROTH M.
	Mon. Not. R. Astron. Soc., 446, 4132-4147 (2015)
	Hubble Frontier Fields: the geometry and dynamics of the massive galaxy cluster merger MACSJ0416.1-2403.
o	Table 2: <[JJE2015] CN> (Nos C1-C2). Fig. 6, Table 3: <[JJE2015] SN> (Nos S1-S2). Fig. 6, Paragr. 6.3.1: <[JJE2015] XN> (Nos X1-X2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JJK2007]
[JJK2007]	(Jorgensen+Johnstone+Kirk+, 2007)
Write:	<<[JJK2007] NN>>
N:	49
Object:	YSO (SIMBAD class: YSO = Young Stellar Object)
Stat:	is completely incorporated in Simbad
Note:	Spitzer Space Telescope Mid-IR observations of the Perseus Molecular Cloud.
in source:	NAME Perseus Molecular Cloud
Ref:	=2007ApJ...656..293J
by	JORGENSEN J.K. , JOHNSTONE D., KIRK H., MYERS P.C.
	Astrophys. J., 656, 293-305 (2007)
	Current star formation in the Perseus molecular cloud: constraints from unbiased submillimeter and mid-infrared surveys.
o	Table 3: <[JJK2007] NN> (Nos 1-49). Table 3: <[BC86b] LDN 1455 IRS N> (No. 4) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JJK2008]
[JJK2008]	(Jorgensen+Johnstone+Kirk+, 2008)
Write:	<<[JJK2008] JHHMMSS.ss+DDMMSS.s>> <<[JJK2008] SMM JHHMMSS+DDMMm>>
N:	44+66
Object:	Poss. YSO + (smm) (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Note:	JCMT SCUBA and Spitzer IRAC and MIPS observations of the Oph Molecular Cloud. N=48 YSO candidate and N=66 submm sources are found.
in source:	NAME rho Oph Cloud
Ref:	=2008ApJ...683..822J
by	JORGENSEN J.K. , JOHNSTONE D., KIRK H., MYERS P.C., ALLEN L.E., SHIRLEY Y.L.
	Astrophys. J., 683, 822-843 (2008)
	Current star formation in the Ophiuchus and Perseus molecular clouds: constraints and comparisons from unbiased submillimeter and mid-infrared surveys. II.
o	Tables 1, 3-4: <[JJK2008] JHHMMSS.ss+DDMMSS.s> N=27+11+6. Table7: <[JJK2008] SMM JHHMMSS+DDMMm> N=66.
=E=	Catalogue in electronic form as <J/ApJ/683/822/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JJK2012]
[JJK2012]	(Jauzac+Jullo+Kneib+, 2012)
Write:	<<[JJK2012] JHHMMSS.sss+DDMMSS.ss>>
N:	2
Object:	Group of G (SIMBAD class: GroupG = Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	Chandra observations of N=2 groups of galaxies, satellites of the cluster MCS J0717.5+3745.
Ref:	=2012MNRAS.426.3369J
by	JAUZAC M. , JULLO E., KNEIB J.-P., EBELING H., LEAUTHAUD A., MA C.-J., LIMOUSIN M., MASSEY R., RICHARD J.
	Mon. Not. R. Astron. Soc., 426, 3369-3384 (2012)
	A weak lensing mass reconstruction of the large-scale filament feeding the massive galaxy cluster MACS J0717.5+3745.
o	Fig. 7, Paragr. 5.1: <[JJK2012] JHHMMSS.sss+DDMMSS.ss> N=2.
o	MACS J0717.5+3749 (abstract & Fig.8) is a misprint for MACS J0717.5+3745.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JJO
JJO	(James+Jeffries, Optical source) (Not yet in Simbad)
Write:	<<JJO NNNN>>
N:	about 1500
Object:	* in Cl* (SIMBAD class: Star)
Note:	I and collaborators have recently completed a multi-wavelength survey in NGC 6475 (M7), a southern open cluster. I have produced a catalogue of some 80,000 stars within 1 degree of the cluster centre with BVI photometry and astrometry with J2000.0 positions accurate to ± 0.2 arcsecs. I plan to publish a subset of the data for those stars which lie with ± one magnitude of the nominal cluster main-sequence. I have been awarded telescope time in june 2002 to measure the radial velocities of each of these photometric members, to confirm cluster membership. The number of stars in the final catalogue is of the order of 1200. The original survey I started in the 90s, was published in MNRAS 1997, 292, 252, Cl* NGC 6475 JJ and detailed the optical and X-ray properties of some 35 or so members of the M7 cluster. I now wish to catalogue a more complete optical data-set based on the original James and Jeffries work.
Auth.:	JAMES D.+
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [JJW2003]
[JJW2003]	(Jakobsen+Jansen+Wagner+, 2003)
Write:	<<[JJW2003] QSO HHMMm+DDMM>>
N:	4
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	VLT FORS observations. Discovery of QSOs near the line of sight of QSO 0302-003, and other foreground QSOs. See also [WW2006].
Ref:	=2003A&A...397..891J
by	JAKOBSEN P. , JANSEN R.A., WAGNER S., REIMERS D.
	Astron. Astrophys., 397, 891-898 (2003)
	Caught in the act: A helium-reionizing quasar near the line of sight to Q0302-003.
o	<[JJW2003] QSO HHMMm+DDMM> N=2.
Ref:	=2006A&A...450..495W
by	WORSECK G. , WISOTZKI L.
	Astron. Astrophys., 450, 495-508 (2006)
	Quasars near the line of sight towards Q 0302-003 and the transverse proximity effect.
o	Table 3, col(1): <[JJW2003] QSO HHMMm+DDMM> N=2 added. Table 3, col(2): <[WW2006] A> (Nos A-F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JK2001]
[JK2001]	(Jahan-Miri+Khosrohahi, 2001) (Not yet in Simbad)
Write:	<<[JK2001] NN>> <<[JK2001] NN'>>
N:	12+2
Object:	Knot (SIMBAD class: PartofG = Part of a Galaxy)
in source:	NGC 7733
Ref:	=2001AJ....122..792J
by	JAHAN MIRI M. , KHOSROSHAHI H.G.
	Astron. J., 122, 792-796 (2001)
	Star formation in the interacting pair NGC 7733/7734.
o	Table 1, Fig.1: <[JK2001] NN> (Nos 1-12, 19-29), <[JK2001] N'> (Nos 5', 6').
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JK2019]
[JK2019]	(Jin+Kong, 2021) (Not yet in Simbad)
Write:	<<[JK2019] NN>>
N:	55
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS observations of N=55 X-ray sources in the field of NGC 7331.
in source:	NGC 7331
Ref:	=2019ApJ...879..112J
by	JIN R. , KONG A.K.H.
	Astrophys. J., 879, 112-112 (2019)
	A multi-epoch X-ray study of the spiral galaxy NGC 7331.
o	Table 2: <[JK2019] NN> (Nos 1-55).
=E=	Catalogue in electronic form as <J/ApJ/879/112/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JKB
JKB	(James Koposov Belokurov)
Write:	<<JKB NNN>>
N:	150
Object:	LSB/SBG (SIMBAD class: Galaxy)
Note:	We have a sample of ∼150 newly discovered dwarf galaxies ("Blue Diffuse Dwarfs"), detected by their morphological properties in the SDSS survey. Each object is a blue, star-forming galaxy, with HII regions embedded within a diffuse continuum. Full details of our project can be found here: http://adsabs.harvard.edu/abs/2015MNRAS.448.2687J
Notes:	The paper 2015MNRAS.448.2687J lists 12 of our sample with spectroscopic observations. Within this publication they are listed as 'KJ objects' but we have been contacted by Marion Schmitz from NED to say that this acronym was already in use. We are now changing KJ to JKB. Our next paper - in-prep and to be submitted in August 2016 - lists a larger sample of 50. We expect the sample to grow, as we use our detection algorithms on new survey data (e.g. DES in the southern hemisphere).
Ref:	=2015MNRAS.448.2687J
by	JAMES B.L. , KOPOSOV S., STARK D.P., BELOKUROV V., PETTINI M., OLSZEWSKI E.W.
	Mon. Not. R. Astron. Soc., 448, 2687-2703 (2015)
	Uncovering blue diffuse dwarf galaxies.
o	Fig. 1, Table 1: <JKB NN> N=12 among (Nos 1-80).
Ref:	=2017MNRAS.465.3977J
by	JAMES B.L. , KOPOSOV S.E., STARK D.P., BELOKUROV V., PETTINI M., OLSZEWSKI E.W., McQUINN K.B.W.
	Mon. Not. R. Astron. Soc., 465, 3977-4015 (2017)
	Blue diffuse dwarf galaxies: a clearer picture.
o	Table 1: <JKB NNN> N=39 added among (Nos 1-144). Institute of Astronomy, Cambridge
=E=	Catalogue in electronic form as <J/MNRAS/448/2687/>
=E=	Catalogue in electronic form as <J/MNRAS/465/3977/>
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [JKC2006]
[JKC2006]	(Jha+Kirshner+Challis+, 2006)
Write:	<<[JKC2006] SN YYYYAA NN>>
N:	425
Object:	* (SIMBAD class: Star)
Note:	FLWO 1.2m telescope observations. Reference stars around 44 SN.
Ref:	=2006AJ....131..527J
by	JHA S. , KIRSHNER R.P., CHALLIS P., GARNAVICH P.M., MATHESON T., SODERBERG A.M., GRAVES G.J.M., HICKEN M., ALVES J.F., ARCE H.G., BALOG Z., BARMBY P., BARTON E.J., BERLIND P., BRAGG A.E., BRICENO C., BROWN W.R., BUCKLEY J.H., CALDWELL N., CALKINS M.L., CARTER B.J., CONCANNON K.D., DONNELLY R.H., ERIKSEN K.A., FABRICANT D.G., FALCO E.E., FIORE F., GARCIA M.R., GOMEZ M., GROGIN N.A., GRONER T., GROOT P.J., HAISCH K.E.Jr, HARTMANN L., HERGENROTHER C.W., HOLMAN M.J., HUCHRA J.P., JAYAWARDHANA R., JERIUS D., KANNAPPAN S.J., KIM D.-W., KLEYNA J.T., KOCHANEK C.S., KORANYI D.M., KROCKENBERGER M., LADA C.J., LUHMAN K.L., LUU J.X., MACRI L.M., MADER J.A., MAHDAVI A., MARENGO M., MARSDEN B.G., McLEOD B.A., McNAMARA B.R., MEGEATH S.T., MORARU D., MOSSMAN A.E., MUENCH A.A., MUNOZ J.A., MUZEROLLE J., NARANJO O., NELSON-PATEL K., PAHRE M.A., PATTEN B.M., PETERS J., PETERS W., RAYMOND J.C., RINES K., SCHILD R.E., SOBCZAK G.J., SPAHR T.B., STAUFFER J.R., STEFANIK R.P., SZENTGYORGYI A.H., TOLLESTRUP E.V., VAISANEN P., VIKHLININ A., WANG Z., WILLNER S.P., WOLK S.J., ZAJAC J.M., ZHAO P., STANEK K.Z.
	Astron. J., 131, 527-554 (2006)
	UBVRI light curves of 44 type Ia supernovae.
o	Table 1 : Anonymous host galaxy of SN 1997DG is [QQH97b] J234014.21+261211.8 in SIMBAD
o	Table 2: <[JKC2006] SN YYYYAA NN> N=425.
=E=	Catalogue in electronic form as J/AJ/131/527
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JKCS
JKCS	(J-K Color Selected)
Write:	<<JKCS NNN>>
Object:	Cluster of G (SIMBAD class: ClG = Cluster of Galaxies)
Note:	In preparation. J-K Colour Selected. Clusters detected as localized overdensities of galaxies of a given colour in the XMM-LSS sky region. See also grCS, RzCS, zKCS. The list of a few public clusters is at: http://www.brera.mi.astro.it/~andreon/clusters_p_ublic.htmlbr First reference with a JKCS cluster: 2009A&A...507..147A.
Auth.:	ANDREON S.
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [JKH2016]
[JKH2016]	(Jose+Kim+Herczeg+, 2016)
Write:	<<[JKH2016] DDD.dddd+DD.dddd>>
N:	9720
Object:	(NIR) (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:	KPNO Mayall 4m NEWFIRM (NOAO Extremely Wide-Field Infrared Imager) near-IR photometric observations of N=9720 sources in the field of AFGL 333 Cloud. Use of archival Spitzer IRAC and MIPS data.
in source:	NAME AFGL 333 Cloud
Ref:	=2016ApJ...822...49J
by	JOSE J. , KIM J.S., HERCZEG G.J., SAMAL M.R., BIEGING J.H., MEYER M.R., SHERRY W.H.
	Astrophys. J., 822, 49-49 (2016)
	Star formation in W3–AFGL 333: young stellar content, properties, and roles of external feedback.
o	Table 3: <[JKH2016] DDD.dddd+DD.dddd> N=9720.
=E=	Catalogue in electronic form as J/ApJ/822/49
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JKK2007]
[JKK2007]	(Jarrett+Koribalski+Kraan-Korteweg+, 2007)
Write:	<<[JKK2007] GN>>
N:	2
Object:	HI G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC MIR, 1.4m IRSF (South Africa) NIR, and ATCA HI observations of 2 galaxies in the Great Attractor Wall.
in source:	NAME Great Attractor
Ref:	=2007AJ....133..979J
by	JARRETT T.H. , KORIBALSKI B.S., KRAAN-KORTEWEG R.C., WOUDT P.A., WHITNEY B.A., MEADE M.R., BABLER B., CHURCHWELL E., BENJAMIN R.A., INDEBETOUW R.
	Astron. J., 133, 979-986 (2007)
	Discovery of two galaxies deeply embedded in the Great Attractor wall.
o	Calibrator PKS 1338-58 not identified.
o	Table 2: <[JKK2007] GN> (Nos G1-G2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JKK2012]
[JKK2012]	(Jung+Ko+Kim+, 2012)
Write:	<<[JKK2012] NNNN>>
N:	1550 (SIMBAD class: C*_Candidate = Carbon Star Candidate)
Note:	CFHT WIRCam NIR observations of NGC 205.
in source:	NGC 205
Ref:	=2012A&A...543A..35J
by	JUNG M.Y. , KO J., KIM J.-W., CHUN S.-H., KIM H.-I., SOHN Y.-J.
	Astron. Astrophys., 543A, 35-35 (2012)
	Near-infrared properties of asymptotic giant branch stars in nearby dwarf elliptical galaxy NGC 205.
o	<[JKK2012] NNNN> N=1550
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JKK96]
[JKK96]	(Jung+Koo+Kang, 1996)
Write:	<<[JKK96] A>>
N:	4
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
in source:	[S87c] Loop 235-3
Ref:	=1996AJ....112.1625J
by	JUNG J.-H. , KOO B.-C., KANG Y.-H.
	Astron. J., 112, 1625-1635 (1996)
	GS 234-02: a star forming supershell in the outer Galaxy.
o	GS 234-02 = part of [S87c] Loop 235-3
o	Table 3: <[JKK96] A> (Nos A-D)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JKM2001]
[JKM2001]	(Johnson+Kobulnicky+Massey+, 2001)
Write:	<<[JKM2001] NGC 6946 NN>> <<[JKM2001] M 33 NN>> <<[JKM2001] NGC 253 N>>
N:	16+14+5
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Search for Ultra Dense (UD) HII candidates in NGC 6946, M 33, NGC 253. Finding charts in Figs 1-3.
in source:	NGC 6946
in source:	M 33 = NGC 598
in source:	NGC 253
Ref:	=2001ApJ...559..864J
by	JOHNSON K.E. , KOBULNICKY H.A., MASSEY P., CONTI P.S.
	Astrophys. J., 559, 864-877 (2001)
	A sample of clusters of extragalactic ultracompact H II regions.
o	Tables 1, 4: <[JKM2001] NGC 6946 NN> (Nos 1-16). Tables 2, 5: <[JKM2001] M 33 NN> (Nos 1-14). Tables 3, 6: <[JKM2001] NGC 253 N> (Nos 1-5).
=E=	Catalogue in electronic form as J/ApJ/559/864
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JKS2008]
[JKS2008]	(Joshi+Kumar+Singh+, 2008)
Write:	<<[JKS2008] NNNN>> <<[JKS2008] XNN>>
N:	1817+66
Object:	(Opt) + (X) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	UBVRIHalpha CCD photometric observations of NGC 7419 with the 104-cm Sampurnanand telescope (Nainital), combined with archival 2MASS and XMM data.
in source:	NGC 7419
Ref:	=2008MNRAS.391.1279J
by	JOSHI H. , KUMAR B., SINGH K.P., SAGAR R., SHARMA S., PANDEY J.C.
	Mon. Not. R. Astron. Soc., 391, 1279-1300 (2008)
	Multiwavelength study of a young open cluster NGC7419.
o	Table 9: ID 44 is a misprint for ID 42 ([JKS2008] 42 in SIMBAD). In ref. list Dobashi + 2005 is 2005PASJ.57... instead of 2005PASP.57...
o	Table 3: <[JKS2008] NNNN> (Nos 1-1817). Table 13: <[JKS2008] XNN> (Nos X1-X66).
=E=	Catalogue in electronic form as J/MNRAS/391/1279
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JKY2018]
[JKY2018]	(Joo+Kyeong+Yang+, 2018)
Write:	<<[JKY2018] VNN>>
N:	97
Object:	RR Lyr (SIMBAD class: RRLyrae = RR Lyrae Variable)
Stat:	is completely incorporated in Simbad
Note:	CTIO 1.6m telescope photometric observations of N=97 RR Lyrae variable stars in the field of Crater II dwarf galaxy.
in source:	NAME Crater II
Ref:	=2018ApJ...861...23J
by	JOO S.-J. , KYEONG J., YANG S.-C., HAN S.-I., SUNG E.-C., KIM D., JEONG H., REE C.H., REY S.-C., JERJEN H., KIM H.-S., CHA S.-M., LEE Y.
	Astrophys. J., 861, 23-23 (2018)
	RR Lyrae variables in the Crater II dwarf galaxy.
o	Table 1: <[JKY2018] VNNN> (Nos 1-97).
=E=	Catalogue in electronic form as <J/ApJ/861/23/>
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: JL
JL	(Jaidee+Lynga)
Write:	<<JL NNN>>
N:	296
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Ref:	=1974ArA.....5..345J
by	JAIDEE S. , LYNGA G.
	Arkiv for Astron., 5, 345-379 (1974)
	A search for faint violet stars in Southern galactic latitudes.
o	JL 181 is L 218-28, not 128-28. Finding charts.
o	<JL NNN> (Nos 1-296)
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [JL81]
[JL81]	(Jacoby+Lesser, 1981) (Not yet in Simbad)
Write:	<<[JL81] IC 10 PN>> <<[JL81] Leo A PNN>> <<[JL81] Sextans A PN>> <<[JL81] Pegasus Galaxy PN>> <<[JL81] WLM PNN>>
N:	1+2+1+1+2
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	PN in dwarf galaxies.
in source:	IC 10
in source:	NAME Leo A
in source:	NAME Sextans A
in source:	NAME Pegasus Galaxy
in source:	DDO 221 = WLM Galaxy
Ref:	=1981AJ.....86..185J
by	JACOBY G.H. , LESSER M.P.
	Astron. J., 86, 185-192 (1981)
	Distances to nearby galaxies derived from planetary nebulae.
o	Figs 1-5: <[JL81] IC 10 PN>, <[JL81] Leo A PN1>, <[JL81] Leo A PN2>, <[JL81] Sextans A PN>, <[JL81] Pegasus Galaxy PN>, <[JL81] WLM PN1>,<[JL81] WLM PN2>.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JLG2019]
[JLG2019]	(Juarez+Liu+Girart+, 2019)
Write:	<<[JLG2019] SMANa>>
N:	6+13
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	SMA 1.3mm continuum observations of N=6 dense cores and N=13 compact millimeter sources in the infrared dark cloud LDN 1287.
in source:	LDN 1287
Ref:	=2019A&A...621A.140J
by	JUAREZ C. , LIU H.B., GIRART J.M., PALAU A., BUSQUET G., GALVAN-MADRID R., HIRANO N., LIN Y.
	Astron. Astrophys., 621A, 140-140 (2019)
	Extreme fragmentation and complex kinematics at the center of the L1287 cloud.
o	Fig. 2, Table 2: <[JLG2019] SMANa> (Nos SMA1-SMA6, SMA3a-SMA3i, SMA5a-SMA5b, SMA6a-SMA6b).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JM99]
[JM99]	(Jamrozy+Machalski, 1999) (Not yet in Simbad)
Write:	<<[JM99] N>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Note:	N=2 possible galaxy identifications of GB2 0909+353.
Ref:	=1999AcA....49..181J
by	JAMROZY M. , MACHALSKI J.
	Acta Astron., 49, 181-188 (1999)
	GB2 0909+353 : one of the largest double radio source.
o	Fig.1: <[JM99] N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JMB2008]
[JMB2008]	(Johns-Krull+McCullough+Burke+, 2008) (Not yet in Simbad)
Write:	<<[JMB2008] N>>
N:	8
Object:	* (SIMBAD class: Star)
Note:	Stars in the field of XO 3.
Ref:	=2008ApJ...677..657J
by	JOHNS-KRULL C.M. , McCULLOUGH P.R., BURKE C.J., VALENTI J.A., JANES K.A., HEASLEY J.N., PRATO L., BISSINGER R., FLEENOR M., FOOTE C.N., GARCIA-MELENDO E., GARY B.L., HOWELL P.J., MALLIA F., MASI G., VANMUNSTER T.
	Astrophys. J., 677, 657-670 (2008)
	XO-3b: a massive planet in an eccentric orbit transiting an F5 V star.
o	Table 2, Fig.1: <[JMB2008] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JMB2018]
[JMB2018]	(Jones+Maclay+Boyer+, 2018)
Write:	<<[JMB2018] LeoA NNN>>
N:	779
Object:	* (SIMBAD class: Star)
Note:	WIYN 3.5-m telescope High Resolution Infrared Camera (WHIRC) JHK photometric observations of N=779 stars in Sextans A and Leo A.
in source:	Sextans A = DDO 75
in source:	NAME Leo A
Ref:	=2018ApJ...854..117J
by	JONES O.C. , MACLAY M.T., BOYER M.L., MEIXNER M., McDONALD I., MESKHIDZE H.
	Astrophys. J., 854, 117-117 (2018)
	Near-infrared stellar populations in the metal-poor, dwarf irregular galaxies Sextans A and Leo A.
o	Table 6: <[JMB2018] LeoA NNN> N=287 among (Nos 0-461), <[JMB2018] SextansA NNN> (Nos 0-491).
=E=	Catalogue in electronic form as J/ApJ/854/117
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JMC2019]
[JMC2019]	(Johnson+Mulchaey+Chen+, 2019)
Write:	<<[JMC2019] JHHMMSS.ss+DDMMSS.s>> <<[JMC2019] 1ES1553+113 group>>
N:	940+1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Magellan telescopes spectroscopy, Mayall telescope MOSAIC and HST ACS imaging of N=940 galaxies in the field of blazar 1ES 1553+113 and of N=1 balzar host group. Use of HST COS archival data.
Ref:	=2019ApJ...884L..31J
by	JOHNSON S.D. , MULCHAEY J.S., CHEN H.-W., WIJERS N.A., CONNOR T., MUZAHID S., SCHAYE J., CEN R., CARLSTEN S.G., CHARLTON J., DROUT M.R., GOULDING A.D., HANSEN T.T., WALTH G.L.
	Astrophys. J., 884L, 31-31 (2019)
	The physical origins of the identified and still missing components of the warm-hot intergalactic medium: insights from deep surveys in the field of blazar 1ES1553+113.
o	Paragr. 3: <[JMC2019] 1ES1553+113 group> N=1. Table 1: <[JMC2019] JHHMMSS.ss+DDMMSS.s> N=940.
=E=	Catalogue in electronic form as <J/ApJ/884/L31/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JME2019]
[JME2019]	(Jauzac+Mahler+Edge+, 2019)
Write:	<<[JME2019] MACS J0417 ANN>> <<[JME2019] MACS J0417 BCG>> <<[JME2019] MACS J0417 1m.N>>
N:	24+1+3
Object:	G + G in Cluster of G + Brightest Cluster Galaxy + Grav. lensed image (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	VLT MUSE observations of N=2 foreground objects, N=14+1 cluster members, and N=8 background galaxies in the core of the massive galaxy cluster MCS J0417.5-1154. N=3 gravitationally lensed images, in addition to the [MSF2019] images. Use of HST (RELICS), Chandra, and VLT SINFONI archival data.
in source:	MCS J0417.5-1154
Ref:	=2019MNRAS.483.3082J
by	JAUZAC M. , MAHLER G., EDGE A.C., SHARON K., GILLMAN S., EBELING H., HARVEY D., RICHARD J., HAMER S.L., FUMAGALLI M., SWINBANK A.M., KNEIB J.-P., MASSEY R., SALOME P.
	Mon. Not. R. Astron. Soc., 483, 3082-3097 (2019)
	The core of the massive cluster merger MACS J0417.5-1154 as seen by VLT/MUSE.
o	Tables 1-3: <[JME2019] MACS J0417 ANN> (Nos F1-F2, G1-G14, B1-B8), <[JME2019] MACS J0417 BCG> N=1. Table 5: <[MSF2019] MACS J0417 NNa.N> (No. 1b.4) added, <[JME2019] MACS J0417 1m.N> (Nos 1m.1-1m.3).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JMG
JMG	(Jones+Miller+Glazebrook)
Write:	<<JMG HHMM+DDMM>> <<JMG HHMM+DDMMA>> <<JMG HHMM+DDMMAA>>
N:	3
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	JMG 0918-0023 = JMG 0918-0023AB
Ref:	=1994MNRAS.270L..47J
by	JONES H.R.A. , MILLER L., GLAZEBROOK K.
	Mon. Not. R. Astron. Soc., 270, 47-51 (1994)
	A new candidate brown dwarf from an infrared survey.
o	<JMG HHMM-DDMMA> N=3
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: JMG99
JMG99	(J.M. Girart+) (Not yet in Simbad)
*****	Avoid the usage of JMG99, prefer [GEH2000]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [JMH2012]
[JMH2012]	(JEE+MAHDAVI+HOEKSTRA+, 2012)
Write:	<<[JMH2012] PN>>
N:	6
Object:	galaxy cluster dark matter substructure (SIMBAD class: ClG = Cluster of Galaxies)
Note:	Hubble Space Telescope/Wide Field Planetary Camera 2 weak-lensing study of ACO 520 to study the substructure of the galaxy cluster.
Ref:	=2012ApJ...747...96J
by	JEE M.J. , MAHDAVI A., HOEKSTRA H., BABUL A., DALCANTON J.J., CARROLL P., CAPAK P.
	Astrophys. J., 747, 96 (2012)
	A study of the dark core in A520 with the Hubble space telescope: the mystery deepens.
o	Table 1: <[JMH2012] PN> N=6 (Nos P1-P6)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JMK2016]
[JMK2016]	(Javanmardi+Martinez-Delgado+Kroupa+, 2016)
Write:	<<[JMK2016] NGC NNNN-DGSAT-N>>
N:	15+13
Object:	LBG (SIMBAD class: LowSurfBrghtG = Low Surface Brightness Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Identification of N=15 low surface brightness (LSB) galaxies in the fields of the nearby galaxies NGC 2683, NGC 3625, NGC 3628, NGC 3669, NGC 4594 (M 104), NGC 4631, NGC 5457 (M 101), and NGC 7814. The format 'DGSAT' stands for Dwarf Galaxy Survey with Amateur Telescopes.
Ref:	=2016A&A...588A..89J
by	JAVANMARDI B. , MARTINEZ-DELGADO D., KROUPA P., HENKEL C., CRAWFORD K., TEUWEN K., GABANY R.J., HANSON M., CHONIS T.S., NEYER F.
	Astron. Astrophys., 588A, 89-89 (2016)
	DGSAT: Dwarf Galaxy Survey with Amateur Telescopes.
o	Table 3: <[JMK2016] NGC NNNN-DGSAT-N> N=15.
Ref:	=2017A&A...603A..18H
by	HENKEL C. , JAVANMARDI B., MARTINEZ-DELGADO D., KROUPA P., TEUWEN K.
	Astron. Astrophys., 603A, 18-18 (2017)
	DGSAT: Dwarf Galaxy Survey with Amateur Telescopes. II. A catalogue of isolated nearby edge-on disk galaxies and the discovery of new low surface brightness systems.
o	Tables 3-4: <[JMK2016] NGC NNNN-DGSAT-N> N=4+4+5 added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JMK2017]
[JMK2017]	(Joseph+Maccarone+Kraft+, 2017) (Not yet in Simbad)
Write:	<<[JMK2017] DDD.ddddd+DD.ddddd>>
N:	238
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS-S observations of N=238 X-ray point sources in the field of the galaxy NGC 4472 in the Virgo cluster. Use of archival Chandra data.
in source:	NGC 4472 = M 49
in source:	NAME Virgo Cluster
Ref:	=2017MNRAS.470.4133J
by	JOSEPH T.D. , MACCARONE T.J., KRAFT R.P., SIVAKOFF G.R.
	Mon. Not. R. Astron. Soc., 470, 4133-4144 (2017)
	A deeper look at the X-ray point source population of NGC 4472.
o	Table 3: <[JMK2017] DDD.ddddd+DD.ddddd> N=238.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JML2000]
[JML2000]	(Juvela+Mattila+Lemke, 2000)
Write:	<<[JML2000] EBLNN N>> <<[JML2000] Mrk314 N>> <<[JML2000] NGP NN>> <<[JML2000] VCN,VCS NN>> <<[JML2000] ZWIIb N>>
N:	55
Object:	(FIR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	ISOPHOT Cosmic Infrared Radiation project. Table 3: N=55 (FIR) in 6 fields (described in T.1).
Ref:	=2000A&A...360..813J
by	JUVELA M. , MATTILA K., LEMKE D.
	Astron. Astrophys., 360, 813-832 (2000)
	Far infrared extragalactic background radiation. I. Source counts with ISOPHOT.
o	Table 3: <[JML2000] EBL22 N> (Nos 1-6), <[JML2000] EBL26 N> (Nos 1-9), <[JML2000] Mrk314 N> (Nos 1-3), <[JML2000] NGP NN> (Nos 1-25), <[JML2000] VCN NN> (Nos 1-10), <[JML2000] ZWIIb N> (Nos 1-2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JML2007]
[JML2007]	(Jeltema+Mulchaey+Lubin+, 2007)
Write:	<<[JML2007] JHHMMSS.ss+DDMMSS.s>>
N:	335
Object:	* in ClG (SIMBAD class: GtowardsCl = Galaxy towards a Cluster of Galaxies)
Note:	Gemini GMOS and KeckI LRIS observations of galaxies in 7 X-ray group of galaxies.
in source:	RX J0329.0+0256
in source:	RX J0720.0+7109
in source:	RX J1205.0+4429
in source:	RX J1256.0+2556
in source:	RX J1334.0+3750
in source:	RX J1347.0+0752
in source:	RX J1648.0+6019
Ref:	=2007ApJ...658..865J
by	JELTEMA T.E. , MULCHAEY J.S., LUBIN L.M., FASSNACHT C.D.
	Astrophys. J., 658, 865-883 (2007)
	The evolution of galaxies in X-ray-luminous groups.
o	RX J1334.0+3750 is a misprint for RX J1334.9+3750. Fig. 8 : galaxies NNN dans ClG J1648+6019 not identified
o	Table 1: <[JML2007] JHHMMSS.ss+DDMMSS.s> N=25+24+54+62+47+43+60.
=E=	Catalogue in electronic form as J/ApJ/658/865
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JML2019]
[JML2019]	(Jameson+McClure-Griffiths+Liu+, 2019) (Not yet in Simbad)
Write:	<<[JML2019] JHHMMSS+DDMMSS>> <<[JML2019] HHMMSS+DDMMSS>> (not recognised by Simbad, but found in literature)
N:	55
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	ATCA observations of N=55 continuum sources in the SMC.
in source:	Magellanic Clouds:SMC = SMC
Ref:	=2019ApJS..244....7J
by	JAMESON K.E. , McCLURE-GRIFFITHS N.M., LIU B., DICKEY J.M., STAVELEY-SMITH L., STANIMIROVIC S., DEMPSEY J., DAWSON J.R., DENES H., BOLATTO A.D., LI D., WONG T.
	Astrophys. J., Suppl. Ser., 244, 7-7 (2019)
	An ATCA survey of H I absorption in the Magellanic Clouds. I. H I gas temperature measurements in the Small Magellanic Cloud.
o	Table 1: <[JML2019] JHHMMSS+DDMMSS> N=55.
=E=	Catalogue in electronic form as <J/ApJS/244/7/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JMM2000]
[JMM2000]	(Junor+Mantovani+Morganti+, 2000) (Not yet in Simbad)
Write:	<<[JMM2000] 0235-197 ANa>> <<[JMM2000] 1203+043 AN>>
N:	7+5
Object:	Component (SIMBAD class: Radio = Radio Source)
Note:	Radio components of the 2 radio-galaxies PKS 0235-197 and PKS 1203+043.
in source:	PKS 0235-197
in source:	PKS 1203+043
Ref:	=2000A&AS..143..457J
by	JUNOR W. , MANTOVANI F., MORGANTI R., PADRIELLI L.
	Astron. Astrophys., Suppl. Ser., 143, 457-464 (2000)
	VLA polarimetry of two extended radio galaxies.
o	Tables 2, 3: <[JMM2000] 0235-197 ANa> (Nos E, C, W, E1-E2, E1a-E1b), <[JMM2000] 1203+043 AN> (Nos N, S, C, J1-J2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JMM2006]
[JMM2006]	(Johnstone+Matthews+Mitchell+, 2001)= (SMM)
Write:	<<[JMM2006] SMM JHHMMmm+DDMMm>>
N:	57
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	SCUBA observations. N=57 850mu.m clumps in Ori B (South). See also OriBsmm and Paper I: [JFM2001].
in source:	NAME Ori B
Ref:	=2006ApJ...639..259J
by	JOHNSTONE D. , MATTHEWS H., MITCHELL G.F.
	Astrophys. J., 639, 259-274 (2006)
	Large area mapping at 850 µm. IV. Analysis of the clump distribution in the Orion B South molecular cloud.
o	Table 1: <[JMM2006] SMM JHHMMmm+DDMMm> N=57.
=E=	Catalogue in electronic form as J/ApJ/639/259
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JMN89]
[JMN89]	(Johnston+Migenes+Norris, 1989) (Not yet in Simbad)
Write:	<<[JMN89] WWN>> <<[JMN89] Center>>
N:	19+1
Object:	OH Maser (SIMBAD class: Maser)
Note:	OH maser clumps in Orion KL.
in source:	NAME Ori-KL
Ref:	=1989ApJ...341..847J
by	JOHNSTON K.J. , MIGENES V., NORRIS R.P.
	Astrophys. J., 341, 847-856 (1989)
	The spatial distribution of the OH masers in Orion-KL.
o	Table 3: <[JMN89] WWN> (Nos NE1-NE8, NW1-NW8, SW1-SW2, SE1), <[JMN89] Center> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JMO94]
[JMO94]	(Jones+Mergen+Odewahn+, 1994)
Write:	<<[JMO94] NNN>>
N:	219
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	OMC:OMC 2 = OMC 2
Ref:	=1994AJ....107.2120J
by	JONES T.J. , MERGEN J., ODEWAHN S., GEHRZ R.D., GATLEY I., MERRILL K.M., PROBST R., WOODWARD C.E.
	Astron. J., 107, 2120-2130 (1994)
	A near-infrared survey of the OMC2 region.
o	Table 1: <[JMO94] NNN> N=219
=E=	Catalogue in electronic form as J/AJ/107/2120
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JMR88]
[JMR88]	(Jensen+Mould+Reid, 1988) (Not yet in Simbad)
Write:	<<[JMR88] SL 506 NN>>
N:	96
Object:	* in Cl* (SIMBAD class: Star)
Note:	Table 1: N=96 * in the cluster [SL63] 506. In tables 2 and 3, stars are designated as 'Cl* NGC 1795 JMR NNNN' and 'Cl* NGC 1754 JMR NNN'.
in source:	[SL63] 506
Ref:	=1988ApJS...67...77J
by	JENSEN J. , MOULD J., REID N.
	Astrophys. J., Suppl. Ser., 67, 77-83 (1988)
	The continuity of cluster formation in the Large Magellanic Cloud.
o	Table 1: <[JMR88] SL 506 NN> (Nos 1-96). Table 2: <Cl* NGC 1795 JMR NNN> (Nos 1-158). Table 3: <Cl* NGC 1754 JMR NNN> (Nos 1-138).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JMS2014]
[JMS2014]	(Jithesh+Misra+Shalima+, 2014)
Write:	<<[JMS2014] JHHMMSS.ss+DDMMSS.ss>>
N:	46
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS observations of N=46 bright X-ray sources in four elliptical galaxies. Use of archival HST ACS multi-epoch images.
in source:	NGC 1399
in source:	NGC 1427
in source:	NGC 4278
in source:	NGC 4486 = M 87 = Virgo A
Ref:	=2014RAA....14.1251J
by	JITHESH V. , MISRA R., SHALIMA P., JEENA K., RAVIKUMAR C.D., BABU B.R.S.
	RAA, 14, 1251-1263 (2014)
	Long term optical variability of bright X-ray point sources in elliptical galaxies.
o	Tables 2-5: <[JMS2014] JHHMMSS.ss+DDMMSS.ss> N=46.
=E=	Catalogue in electronic form as <J/other/RAA/14.1251/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JMS2020]
[JMS2020]	(Jaelani+More+Sonnenfeld+, 2020)
Write:	<<[JMS2020] HSC J0904-0102 system>> <<[JMS2020] HSC J0904-0102 A>>
N:	1+5
Object:	Grav. lens system + Grav. lensed image + Grav. lens (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Gemini South GMOS observations of N=1 gravitational lens system, consisting of the lens galaxy G and four gravitationally lensed images (A-D). Use of the Subaru Hyper Suprime-Cam (HSC) survey.
Ref:	=2020MNRAS.494.3156J
by	JAELANI A.T. , MORE A., SONNENFELD A., OGURI M., RUSU C.E., WONG K.C., CHAN J.H.H., SUYU S.H., KAYO I., LEE C.-H., INOUE K.T.
	Mon. Not. R. Astron. Soc., 494, 3156-3165 (2020)
	Discovery of an unusually compact lensed Lyman-break galaxy from the Hyper Suprime-Cam Survey.
o	Fig. 1, Table 1: <[JMS2020] HSC J0904-0102 system> N=1, <[JMS2020] HSC J0904-0102 A> (Nos A-D, G).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JMS77]
[JMS77]	(Jorden+MacGregor+Selby+, 1977)= (IRS)
Write:	<<[JMS77] IRS N>>
N:	4
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
in source:	GAL 045.5+00.1
Ref:	=1977MNRAS.181..157J
by	JORDEN P.R. , MacGREGOR A.D., SELBY M.J., WHITELOCK P.A., SANCHEZ MAGRO C.
	Mon. Not. R. Astron. Soc., 181, 157-161 (1977)
	Infrared sources in the compact H2 region G 45.5+0.1.
o	Table 1: <[JMS77] IRS N> (Nos 1-4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JMT2009]
[JMT2009]	(Johnson+Mendez+Teodorescu, 2009)
Write:	<<[JMT2009] NNN>>
N:	7+109
Object:	Poss. PN (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
Note:	Subaru FOCAS observations of M82. Use of HST ACS imaging.
in source:	M82 = NGC 3034
Ref:	=2009ApJ...697.1138J
by	JOHNSON L.C. , MENDEZ R.H., TEODORESCU A.M.
	Astrophys. J., 697, 1138-1152 (2009)
	Discovery, photometry, and kinematics of planetary nebulae in M 82.
o	Tables 2-3: <[JMT2009] NNN> N=7+109 among (Nos 101-274).
=E=	Catalogue in electronic form as <J/ApJ/697/1138/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Jn
Jn	(Jones)= (Jones)
Write:	<<PN Jn N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Note:	Jn 1 = PN G104.2-29.6 = PK 104-29 1
Ref:	=1949ApJ...109..537M
by	MILLER F.D. , VAN DIEN E.
	Astrophys. J., 109, 537-538 (1949)
	A large new planetary nebula.
o	(Erratum) erratum ApJ 110, 104 (1949)
o	PN Jn
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [JNB98]
[JNB98]	(Jackson+Nair+Browne+, 1998)
Write:	<<[JNB98] B0712+472 A>>
N:	4+1
Object:	Component + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST All-Sky Survey and CLASS survey. Table 2: The lensing system '[FC98] B0712+472' consists of 4 components (Nos A-D), and a lensing galaxy 'G'. See also [FC98]
in source:	CLASS B0712+472
Ref:	=1998MNRAS.296..483J
by	JACKSON N. , NAIR S., BROWNE I.W.A., WILKINSON P.N., MUXLOW T.W.B., DE BRUYN A.G., KOOPMANS L., BREMER M., SNELLEN I., MILEY G.K., SCHILIZZI R.T., MYERS S., FASSNACHT C.D., WOMBLE D.S., READHEAD A.C.S., BLANDFORD R.D., PEARSON T.J.
	Mon. Not. R. Astron. Soc., 296, 483-490 (1998)
	B0712+472: a new radio four-image gravitational lens.
o	Table 2: <[JNB98] B0712+472 A> (Nos A-D), <[JNB98] B0712+472 G> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JnEr
JnEr	(Discoverers: Jones+Emberson)
Write:	<<PN JnEr N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	JnEr 1 = PN G164.8+31.1 = PK 164+31 1
Ref:	=1977PASP...89..261B
by	BARBIERI C. , SULENTIC J.W.
	Publ. Astron. Soc. Pac., 89, 261-263 (1977)
	The planetary nebula 164+31 1.
o	<PN JnEr N> N=1
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [JNK2010]
[JNK2010]	(Jullo+Natarajan+Kneib+, 2010) (Not yet in Simbad)
Write:	<<[JNK2010] NN.Na>>
N:	18
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	N=18 strong lensing features in the field of Abell 1689. See also [BBC2005].
in source:	ACO 1689
Ref:	=2010Sci...329..924J
by	JULLO E. , NATARAJAN P., KNEIB J.-P., D'ALOISIO A., LIMOUSIN M., RICHARD J., SCHIMD C.
	Sci, 329, 924-927 (2010)
	Cosmological constraints from strong gravitational lensing in clusters of galaxies.
o	Table 1: <[JNK2010] NN.Na> N=18 among (Nos 4.1a-24.4b)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JNS2011]
[JNS2011]	(Joshi+Nandi+Saikia+, 2011)
Write:	<<[JNS2011] JHHMMSS.ss+DDMMSS.s>>
N:	320
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	GMRT 154MHz observations of the field of 3C 293.
in source:	3C 293
Ref:	=2011MNRAS.414.1397J
by	JOSHI S.A. , NANDI S., SAIKIA D.J., ISHWARA-CHANDRA C.H., KONAR C.
	Mon. Not. R. Astron. Soc., 414, 1397-1404 (2011)
	A radio study of the double–double radio galaxy 3C293.
o	Table A.1: <[JNS2011] JHHMMSS.ss+DDMMSS.s> N=320.
=E=	Catalogue in electronic form as <J/MNRAS/414/1397/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JNW2009]
[JNW2009]	(Jeffries+Naylor+Walter+, 2009)
Write:	<<[JNW2009] FF NNNN>> <<[JNW2009] FF-NNNN>> (not recognised by Simbad, but found in literature)
N:	86972
Object:	Unknown (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	CTIO 0.9m telescope photometry, CTIO 4m telescope spectroscopy and XMM-Newton observations of the field of Gam Vel.
in source:	NAME ASS VEL OB 2-
Ref:	=2009MNRAS.393..538J
by	JEFFRIES R.D. , NAYLOR T., WALTER F.M., POZZO M.P., DEVEY C.R.
	Mon. Not. R. Astron. Soc., 393, 538-556 (2009)
	The stellar association around γ Velorum and its relationship with Vela OB2.
o	The Stellar association around γ Velorum = Name Gam Vel Subcluster.
o	Table 2: <[JNW2009] FF NNNN> N=86972.
=E=	Catalogue in electronic form as J/MNRAS/393/538
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JNW2014]
[JNW2014]	(Jeon+Nemec+Walker+, 2014)
Write:	<<[JNW2014] NGC NNNN NNNNN>> <<[JNW2014] Reticulum NNN>>
N:	1418+2004+13087+2049+766
Object:	* (SIMBAD class: Star)
Note:	CTIO SMARTS observations of N=19324 stars in and around 5 Magellanic Cloud globular clusters (NGC 1466, NGC 1841, NGC 2210, NGC 2257, and Reticulum).
in source:	NGC 1466
in source:	NGC 1841
in source:	NGC 2210
in source:	NGC 2257
in source:	NAME Reticulum Cluster
Ref:	=2014AJ....147..155J
by	JEON Y.-B. , NEMEC J.M., WALKER A.R., KUNDER A.M.
	Astron. J., 147, 155 (2014)
	B, V photometry for ~19,000 stars in and around the Magellanic Cloud globular clusters NGC 1466, NGC 1841, NGC 2210, NGC 2257, and Reticulum.
o	Tables 4-8: <[JNW2014] NGC NNNN NNNNN> N=1418+2004+13087+2049, <[JNW2014] Reticulum NNN> N=766 among (Nos 5-851).
=E=	Catalogue in electronic form as <J/AJ/147/155/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JNX94]
[JNX94]	(Jarrett+Novak+Xie+, 1994)
Write:	<<[JNX94] HHMMSS.s+DDMMSS>>
N:	114
Object:	* (SIMBAD class: Star)
Note:	No format given by the authors. We use coordinates as format.
in source:	NAME Mon R2 GMC
Ref:	=1994ApJ...430..743J
by	JARRETT T.H. , NOVAK G., XIE T., GOLDSMITH P.F.
	Astrophys. J., 430, 743-756 (1994)
	Magnetic field structure in Monoceros R2.
o	VSS 185 = [VSS88] 185
o	Table 1: <[JNX94] HHMMSS.s+DDMMSS> N=114
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JoDi
JoDi	(Jones+Dickel)
Write:	<<JoDi N>>
N:	1
Object:	Poss. PN (SIMBAD class: PlanetaryNeb_Candidate = Planetary Nebula Candidate)
Note:	The PN is called 'JoDi 1' and considered only as a possible PN in Acker+ 1992ESOPN...1....1A catalogue of PN.
Ref:	=1984BAAS...16..975J
by	JONES E.M. , DICKEL J.R.
	Bull. American Astron. Soc., 16, 975-None (1984)
	The planetary nebula surrounding Tycho's supernova remnant.
o	<JoDi 1> N=1
Origin	of the Acronym: L (1992ESOPN...1....1A)
Details on Acronym: Johansson
Johansson	(Johansson)
Write:	<<Cl Johansson N>>
N:	1
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Ref:	=1981A&AS...44..127J
by	JOHANSSON K.L.V.
	Astron. Astrophys., Suppl. Ser., 44, 127-129 (1981)
	A study of small cluster candidate in Norma.
o	<Cl Johansson 1>. Table 1: <Cl Johansson 1 N> (Nos 1-5).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Johnson
Johnson	(Johnson+)
*****	Avoid the usage of Johnson, prefer Schulte
Origin	of the Acronym: L (1966PROE....5..111R)
Details on Acronym: [JON2007]
[JON2007]	(Jeffries+Oliveira+Naylor+, 2007) (Not yet in Simbad)
Write:	<<[JON2007] N.NN NNNNN>>
N:	27131
Object:	* in Cl* (SIMBAD class: Star)
Note:	Gemini North telescope CCD photometry of NGC 2169.
in source:	NGC 2169
Ref:	=2007MNRAS.376..580J
by	JEFFRIES R.D. , OLIVEIRA J.M., NAYLOR T., MAYNE N.J., LITTLEFAIR S.P.
	Mon. Not. R. Astron. Soc., 376, 580-598 (2007)
	The Keele-Exeter young cluster survey - I. Low-mass pre-main-sequence stars in NGC 2169.
o	Table 3: <[JON2007] N.NN NNNNN> N=27131. Table 5: <Cl* NGC 2169 JON NN> (Nos 1-47).
=E=	Catalogue in electronic form as J/MNRAS/376/580
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Jonckheere
Jonckheere	(Jonckheere)= (J)
Write:	<<Jonckheere NNNN>>
N:	3355
Object:	* (SIMBAD class: Star)
Note:	Jonckheere R., 1962, general catalogue of 3350 faint double stars, observed from 1906 to 1962. Edit. Observatoire de Marseille. Ref. for these objects are collected p. 7 and in the Index, which gives J2000 coordinates. Nebulae, Novae are listed p. 418. For double *, use IDS Nomenclature. Nos 320, 475, 900 are PN.
Ref:	=1916Obs....39..134J
by	JONCKHEERE R.
	The Observatory, 39, 134-135 (1916)
	A new stellar nebula.
o	<Jonckheere NNNN> (Nos 1-3350).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Jones
Jones	(Jones)
*****	Avoid the usage of Jones, prefer Jn
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [JOO2008]
[JOO2008]	(Jackson+Ofek+Oguri, 2008)
Write:	<<[JOO2008] image A>> <<[JOO2008] lensing G>>
N:	2+1
Object:	Grav. lensed image + G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	UKIRT IR Deep Sky Survey and SDSS observations.
Ref:	=2008MNRAS.387..741J
by	JACKSON N. , OFEK E.O., OGURI M.
	Mon. Not. R. Astron. Soc., 387, 741-746 (2008)
	ULAS J234311.93-005034.0: a gravitational lens system selected from UKIDSS and SDSS.
o	Table 1, Fig.5: <[JOO2008] image A> (Nos A-B), <[JOO2008] lensing G> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JOO2009]
[JOO2009]	(Jackson+Ofek+Oguri, 2009)
Write:	<<[JOO2009] ULAS J082016.1+081216 lens>>
N:	1
Object:	Grav. lens (SIMBAD class: GravLens = Gravitational Lens)
Stat:	is completely incorporated in Simbad
Note:	Keck I LRIS observations of N=1 gravitational lens, as part of the Major UKIDSS-SDSS Cosmic Lens Survey (MUSCLES). Use of UKIDSS DR4 and SDSS DR5 data. See also [JOO2008].
Ref:	=2009MNRAS.398.1423J
by	JACKSON N. , OFEK E.O., OGURI M.
	Mon. Not. R. Astron. Soc., 398, 1423-1427 (2009)
	A new gravitational lens from the MUSCLES survey: ULASJ082016.1+081216.
o	<[JOO2009] ULAS J082016.1+081216 lens> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Joshi
Joshi	(Joshi+)
Write:	<<Joshi NN>>
N:	24
Object:	* (SIMBAD class: Star)
Note:	Map in Plate 1
in source:	Barnard 5
Ref:	=1985MNRAS.215..275J
by	JOSHI U.C. , KULKARNI P.V., BHATT H.C., KULSHRESTHA A.K., DESHPANDE M.R.
	Mon. Not. R. Astron. Soc., 215, 275-280 (1985)
	Polarization measurements of stars in the region of Bok globule B5.
o	Table 1: <Joshi NN> (Nos 1-24)
Origin	of the Acronym: L (1997ApJ...491L.103A)
Details on Acronym: JP
JP	(Jodrell Bank, Pulsar)
Rem:	Superseded by PSR
*****	Avoid the usage of JP, prefer PSR
Details on Acronym: JP11
JP11	(Johnson Photometry 11 colors)
Write:	<<JP11 NNNN>>
N:	4494
Object:	* (SIMBAD class: Star)
Note:	Catalog of 5943 measurements for N=4494 stars in multicolour photometry (UBVRIJHKLMN, Johnson et al. 1964BOTT....3..305J and 1968ApJ...152..465J).
Ref:	=1978A&AS...34..477M
by	MOREL M. , MAGNENAT P.
	Astron. Astrophys., Suppl. Ser., 34, 477-None (1978)
	UBVRIJKLMNH Photoelectric Photometric Catalogue.
o	<JP11 NNNN> N=4494 among (Nos 1-5943).
=E=	Catalogue in electronic form as <II/7/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JP2001]
[JP2001]	(Jones+Preston, 2001)
Write:	<<[JP2001] BHHMMSS+DDMM>>
N:	10+19+15+10+17+18
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	Radio-sources in 3 fields 1409+52, 1641+39, 1749+70, at 327Mhz and 74Mhz in each field.
Ref:	=2001AJ....122.2940J
by	JONES D.L. , PRESTON R.A.
	Astron. J., 122, 2940-2953 (2001)
	Fossil radio emission associated with currently active radio galaxies.
o	Tables 1-6: <[JP2001] BHHMMSS+DDMM> N=10+19+15+10+17+18.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JPB2009]
[JPB2009]	(Jordan+Peng+Blakeslee+, 2009)
Write:	<<[JPB2009] DDD.ddddddd+DD.ddddddd>>
N:	12763
Object:	Unknown (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	HST ACS observations. Search for globular cluster candidates in VCC galaxies.
in source:	NAME Virgo Cluster
Ref:	=2009ApJS..180...54J
by	JORDAN A. , PENG E.W., BLAKESLEE J.P., COTE P., EYHERAMENDY S., FERRARESE L., MEI S., TONRY J.L., WEST M.J.
	Astrophys. J., Suppl. Ser., 180, 54-66 (2009)
	The ACS Virgo cluster survey XVI. Selection procedure and catalogs of globular cluster candidates.
o	Table 4, cols(2,3): <[JPB2009] DDD.ddddddd+DD.ddddddd> N=12763.
=E=	Catalogue in electronic form as J/ApJS/180/54
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JPB2015]
[JPB2015]	(Jordan+Peng+Blakeslee+, 2015)
Write:	<<[JPB2015] DDD.ddddddd+DD.ddddddd>>
N:	9136
Object:	Poss. GlCl (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	HST ACS observations of N=9136 globular cluster candidates for 43 galaxies from the ACS Fornax Cluster survey. See also [JPB2009].
in source:	NAME Fornax Cluster
Ref:	=2015ApJS..221...13J
by	JORDAN A. , PENG E.W., BLAKESLEE J.P., COTE P., EYHERAMENDY S., FERRARESE L.
	Astrophys. J., Suppl. Ser., 221, 13 (2015)
	The ACS Fornax Cluster Survey. XI. Catalog of globular cluster candidates.
o	(Erratum) erratum vol. 233, art. 27 (2017)
o	Table 2: <[JPB2015] DDD.ddddddd+DD.ddddddd> N=9136.
=E=	Catalogue in electronic form as J/ApJS/221/13
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JPC2004]
[JPC2004]	(Jamet+Perez+Cervino+, 2004)
Write:	<<[JPC2004] NN>>
N:	56
Object:	* in Cl* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Brightest stars in the ionizing cluster of NGC 588.
in source:	NGC 588
Ref:	=2004A&A...426..399J
by	JAMET L. , PEREZ E., CERVINO M., STASINSKA G., GONZALEZ-DELGADO R.M., VILCHEZ J.M.
	Astron. Astrophys., 426, 399-413 (2004)
	On the importance of the few most massive stars: The ionizing cluster of NGC 588.
o	Table 4: <[JPC2004] NN> (Nos 1-56).
=E=	Catalogue in electronic form as <J/A+A/426/399/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JPF2000]
[JPF2000]	(Jones+Ponman+Forbes, 2000)
Write:	<<[JPF2000] GNN>>
N:	11
Object:	G in Group (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Stat:	is completely incorporated in Simbad
Note:	N=11 galaxies in RX J1340.6+4018 Group.
in source:	NAME RX J13406+4018 GROUP
Ref:	=2000MNRAS.312..139J
by	JONES L.R. , PONMAN T.J., FORBES D.A.
	Mon. Not. R. Astron. Soc., 312, 139-150 (2000)
	Multiwavelength observations of an evolved galaxy group: an end-point of galaxy merging?.
o	Table 1, Fig.1: <[JPF2000] GNN> (Nos G1-G11).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JPF2006]
[JPF2006]	(Jarrett+Polletta+Fournon+, 2006)
Write:	<<[JPF2006] JHHMMSS.ss+DDMMSS.ss>> <<[JPF2006] JHHMMSS.ss+DDMMSS.s>>
N:	2+3
Object:	Star Cluster + Part of G (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	Spitzer Space Telescope IR imaging of UGC 10214: 2 SSC (Super Star Cluster) are found, and 3 star formation hot spots.
in source:	UGC 10214 = Tadpole Galaxy
Ref:	=2006AJ....131..261J
by	JARRETT T.H. , POLLETTA M., FOURNON I.P., STACEY G., XU K., SIANA B., FARRAH D., BERTA S., HATZIMINAOGLOU E., RODIGHIERO G., SURACE J., DOMINGUE D., SHUPE D., FANG F., LONSDALE C., OLIVER S., ROWAN-ROBINSON M., SMITH G., BABBEDGE T., GONZALEZ-SOLARES E., MASCI F., FRANCESCHINI A., PADGETT D.
	Astron. J., 131, 261-281 (2006)
	Remarkable disk and off-nuclear starburst activity in the Tadpole galaxy as revealed by the Spitzer Space Telescope.
o	Text: <[JPF2006] JHHMMSS.ss+DDMMSS.s> N=1+3, <[JPF2006] JHHMMSS.s+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JPJ2000]
[JPJ2000]	(Jurcevic+Pierce+Jacoby, 2000)
Write:	<<[JPJ2000] VNN>>
N:	42
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	N=42 red supergiants in NE and SE field of M 101.
in source:	M 101 = NGC 5457
Ref:	=2000MNRAS.313..868J
by	JURCEVIC J.S. , PIERCE M.J., JACOBY G.H.
	Mon. Not. R. Astron. Soc., 313, 868-880 (2000)
	Period-luminosity relations for red supergiant variables - II. The distance to M 101.
o	in ref list Feast 1980MNRAS.193..377F instead of 193.337
o	Tables 4, 5: <[JPJ2000] VNN> (Nos V1-V42).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JPN2003]
[JPN2003]	(Joshi+Pandley+Narasimha+, 2003)
Write:	<<[JPN2003] VNNN>>
N:	359
Object:	V* (SIMBAD class: Variable* = Variable Star)
Stat:	is completely incorporated in Simbad
Note:	Naini Tal telescope observations. Identification of variable stars in M 31. (Nos 1-26) are Cepheids.
in source:	M 31 = NGC 224
Ref:	=2003A&A...402..113J
by	JOSHI Y.C. , PANDEY A.K., NARASIMHA D., SAGAR R., GIRAUD-HERAUD Y.
	Astron. Astrophys., 402, 113-123 (2003)
	Identification of 13 Cepheids and 333 other variables in M31.
o	Tables 4, 5: <[JPN2003] VNNN> (Nos V1-V359).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JPO2008]
[JPO2008]	(Jose+Pandey+Ojha+, 2008)
Write:	<<[JPO2008] IC 417 NN>>
N:	13
Object:	OB* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Compilation of OB stars in the region of IC 417.
in source:	IC 417
Ref:	=2008MNRAS.384.1675J
by	JOSE J. , PANDEY A.K., OJHA D.K., OGURA K., CHEN W.P., BHATT B.C., GHOSH S.K., MITO H., MAHESWAR G., SHARMA S.
	Mon. Not. R. Astron. Soc., 384, 1675-1700 (2008)
	Stellar contents and star formation in the young open cluster Stock 8.
o	Table 2: <Cl* Stock 8 JPO NNNN> (Nos 1-7924). Table 4: <Cl* Stock 8 JPOHA NN> (Nos 1-25). Table 6: <[JPO2008] IC 417 NN> (Nos 1-13).
=E=	Catalogue in electronic form as <J/MNRAS/384/1675/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JPO2011]
[JPO2011]	(Jose+Pandey+Ogura+, 2011)
Write:	<<[JPO2011] NNNN>>
N:	2425
Object:	* (SIMBAD class: Star)
Note:	Himalayan Chandra 2m telescope (HCT, India) HFOSC (UBVRI photometry and spectroscopy) observations of NGC 1624.
in source:	NGC 1624
Ref:	=2011MNRAS.411.2530J
by	JOSE J. , PANDEY A.K., OGURA K., OJHA D.K., BHATT B.C., SAMAL M.R., CHAUHAN N., SAHU D.K., RAWAT P.S.
	Mon. Not. R. Astron. Soc., 411, 2530-2548 (2011)
	A multiwavelength census of stellar contents in the young cluster NGC 1624.
o	Table 2: <[JPO2011] NNNN> (Nos 1-2425).
=E=	Catalogue in electronic form as <J/MNRAS/411/2530/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JPO2012]
[JPO2012]	(Jose+Pandey+Ogura+, 2012)
Write:	<<[JPO2012] JHHMMSS.ss+DDMMSS.s>> <<[JPO2012] NN>>
N:	61+16
Object:	Halpha emitting source + * (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Himalayan Chandra 2m telescope (HCT, India) HFOSC spectroscopy and Kiso Observatory 105-cm Schmidt Telescope photometry of N=61 Hα emitting sources and N=16 stars in the Sh 2-254 complex.
in source:	SH 2-254
Ref:	=2012MNRAS.424.2486J
by	JOSE J. , PANDEY A.K., OGURA K., SAMAL M.R., OJHA D.K., BHATT B.C., CHAUHAN N., ESWARAIAH C., MITO H., KOBAYASHI N., YADAV R.K.
	Mon. Not. R. Astron. Soc., 424, 2486-2503 (2012)
	Optical and near-infrared survey of the stellar contents associated with the star-forming complex Sh2-252.
o	Table 2: <[JPO2012] JHHMMSS.ss+DDMMSS.s> N=61. Fig. 2, Table 4: <[JPO2012] NN> (Nos 1-16).
Details on Acronym: JPS
JPS	(JCMT Plane Survey)
Write:	<<JPS GLLL.lll+BB.bbb>>
N:	7813
Object:	(smm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Stat:	is completely incorporated in Simbad
Note:	JCMT SCUBA-2 850µm continuum survey of six fields in the northern inner Galactic plane in a longitude range of l=7°-63°. 2017MNRAS.469.2163E: JCMT Plane Survey Public Release 1 (N=7813 sources). See also JCMTLSP
Ref:	=2017MNRAS.469.2163E
by	EDEN D.J. , MOORE T.J.T., PLUME R., URQUHART J.S., THOMPSON M.A., PARSONS H., DEMPSEY J.T., RIGBY A.J., MORGAN L.K., THOMAS H.S., BERRY D., BUCKLE J., BRUNT C.M., BUTNER H.M., CARRETERO D., CHRYSOSTOMOU A., CURRIE M.J., DEVILLIERS H.M., FICH M., GIBB A.G., HOARE M.G., JENNESS T., MANSER G., MOTTRAM J.C., NATARIO C., OLGUIN F., PERETTO N., PESTALOZZI M., POLYCHRONI D., REDMAN R.O., SALJI C., SUMMERS L.J., TAHANI K., TRAFICANTE A., DIFRANCESCO J., EVANS A., FULLER G.A., JOHNSTONE D., JONCAS G., LONGMORE S.N., MARTIN P.G., RICHER J.S., WEFERLING B., WHITE G.J., ZHU M.
	Mon. Not. R. Astron. Soc., 469, 2163-2183 (2017)
	The JCMT Plane Survey: first complete data release - emission maps and compact source catalogue.
o	Table 2, col. 1: <JPS GLLL.lll+BB.bbb> N=7813 = Table 2, col. 2: <JCMTLSP JHHMMSS.s+DDMMSS> N=7813.
=E=	Catalogue in electronic form as <J/MNRAS/469/2163/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: JPS
JPS	(JCMT Plane Survey)
*****	Avoid the usage of JPS, prefer [MPT2015]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [JPV2013]
[JPV2013]	(Jaffe+Poggianti+Verheijen+, 2013)
Write:	<<[JPV2013] IJHHMMSS.ss+DDMMSS.s>>
N:	594
Object:	G (SIMBAD class: Galaxy)
Note:	WHT optical spectroscopy for N=594 galaxies in ACO 963 and ACO 2192, as part of the Blind Ultra Deep HI Environmental Survey (BUDHIES).
in source:	ACO 963
in source:	ACO 2192
Ref:	=2013MNRAS.431.2111J
by	JAFFE Y.L. , POGGIANTI B.M., VERHEIJEN M.A.W., DESHEV B.Z., VAN GORKOM J.H.
	Mon. Not. R. Astron. Soc., 431, 2111-2125 (2013)
	BUDHIES I: characterizing the environments in and around two clusters at z~=0.2.
o	Table C1: <[JPV2013] IJHHMMSS.ss+DDMMSS.s> N=594.
=E=	Catalogue in electronic form as <J/MNRAS/431/2111/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JRB2015]
[JRB2015]	(Johnston+Robitaille+Beuther+, 2015)
Write:	<<[JRB2015] AFGL 4176 mmNNa>> <<[JRB2015] AFGL 4176 mm1-main>>
N:	17+7+1
Object:	(mm) (SIMBAD class: mmRad = Millimetric Radio Source)
Note:	ALMA 1.2mm continuum observations of N=17+7+1 sources in the field of AFGL 4176.
in source:	RAFGL 4176
Ref:	=2015ApJ...813L..19J
by	JOHNSTON K.G. , ROBITAILLE T.P., BEUTHER H., LINZ H., BOLEY P., KUIPER R., KETO E., HOARE M.G., VAN BOEKEL R.
	Astrophys. J., 813L, 19 (2015)
	A keplerian-like disk around the forming O-type star AFGL 4176.
o	Fig. 1: <[JRB2015] AFGL 4176 mmN> (Nos mm1-mm8).
Ref:	=2020A&A...634L..11J
by	JOHNSTON K.G. , HOARE M.G., BEUTHER H., KUIPER R., KEE N.D., LINZ H., BOLEY P., MAUD L.T., AHMADI A., ROBITAILLE T.P.
	Astron. Astrophys., 634L, 11-11 (2020)
	Spiral arms and instability within the AFGL 4176 mm1 disc.
o	Fig. 1: <[JRB2015] AFGL 4176 mm1-main> N=1, <[JRB2015] AFGL 4176 mmNa> (Nos 1a-1d, 6b).
Ref:	=2020ApJ...896...35J
by	JOHNSTON K.G. , HOARE M.G., BEUTHER H., LINZ H., BOLEY P., KUIPER R., KEE N.D., ROBITAILLE T.P.
	Astrophys. J., 896, 35-35 (2020)
	A detailed view of the circumstellar environment and disk of the forming O-star AFGL 4176.
o	Fig. 1, Table 4: <[JRB2015] AFGL 4176 mmNNa> (Nos mm7a-mm7b, mm9-mm17) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JRB99]
[JRB99]	(Jackson+Roland+Bremer+, 1999)
Write:	<<[JRB99] HHMMSS.ss+DDMMSS.s>>
N:	297
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA observations of radio components of 4C sources. See also paper I: [RMW96]
Ref:	=1999A&AS..134..401J
by	JACKSON N. , ROLAND J., BREMER M., RHEE G., WEBB J.
	Astron. Astrophys., Suppl. Ser., 134, 401-436 (1999)
	VLA observations of a 4C equatorial sample. II.
o	Table 2: <[JRB99] HHMMSS.ss+DDMMSS.s> N=297.
=E=	Catalogue in electronic form as J/A+AS/134/401
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JRF2003]
[JRF2003]	(Johnston+Richards+Frieman+, 2003)
Write:	<<[JRF2003] J0903+5028 A>> <<[JRF2003] JHHMMSS+DDMMSS>>
N:	2+1+2
Object:	Grav. lensed image + G + Cluster of G (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	SDSS J090334.92+502819.2 is a lensed QSO candidate, with 2 lensed images A and B. and a lensing galaxy G. N=2 cluster of galaxies are identified in the lens model results.
Ref:	=2003AJ....126.2281J
by	JOHNSTON D.E. , RICHARDS G.T., FRIEMAN J.A., KEETON C.R., STRAUSS M.A., KNAPP G.R., BECKER R.H., WHITE R.L., JOHNSON E.T., MA Z., SUBBARAO M., BAHCALL N.A., BERNARDI M., BRINKMANN J., EISENSTEIN D.J., FUKUGITA M., HALL P.B., INADA N., PINDOR B., SCHLEGEL D.J., SCRANTON R., SHELDON E.S., SCHNEIDER D.P., SZALAY A.S., YORK D.G.
	Astron. J., 126, 2281-2290 (2003)
	SDSS J090334.92+502819.2: a new gravitational lens.
o	Fig.1, Table 2: <[JRF2003] J0903+5028 A> (Nos A-B, G). Table 3: <[JRF2003] JHHMMSS+DDMMSS> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JRJ2015]
[JRJ2015]	(Jauzac+Richard+Jullo+, 2015) (Not yet in Simbad)
Write:	<<[JRJ2015] NN.N>>
N:	173
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	N=173 gravitationally lensed images in 61 systems in the field of the galaxy cluster Abell 2744. Use of HST ACS and WFC3 data from the Hubble Frontier Fields (HFF) project.
in source:	ACCG 118 = ACO 2744
Ref:	=2015MNRAS.452.1437J
by	JAUZAC M. , RICHARD J., JULLO E., CLEMENT B., LIMOUSIN M., KNEIB J.-P., EBELING H., NATARAJAN P., RODNEY S., ATEK H., MASSEY R., ECKERT D., EGAMI E., REXROTH M.
	Mon. Not. R. Astron. Soc., 452, 1437-1446 (2015)
	Hubble Frontier Fields: a high-precision strong-lensing analysis of the massive galaxy cluster Abell 2744 using ~ 180 multiple images.
o	Fig. 1, Table 3: <[JRJ2015] NN.N> N=173 among (Nos 1.1-1.3 to 61.1-61.2).
=E=	Catalogue in electronic form as <J/MNRAS/452/1437/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JRL2006]
[JRL2006]	(Janknecht+Reimers+Lopez+, 2006) (Not yet in Simbad)
Write:	<<[JRL2006] QSO JHHMM+DDMM abs N.NNNNNNN>>
N:	1325
Object:	Absorber
Note:	Statistical properties of Ly-alpha absorber lines in 9 qsoS.
Ref:	=2006A&A...458..427J
by	JANKNECHT E. , REIMERS D., LOPEZ S., TYTLER D.
	Astron. Astrophys., 458, 427-439 (2006)
	The evolution of Lyman α absorbers in the redshift range 0.5<z<1.9.
o	List: <[JRL2006] QSO J1634+7031 abs N.NNNNNNN> N=1325.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JRM2010]
[JRM2010]	(Juvela+Ristocelli+Montier+, 2010)
Write:	<<[JRM2010] PCC288-A>> <<[JRM2010] PCCNNN-PN>>
N:	5+4
Object:	Core (SIMBAD class: denseCore = Dense Core)
Note:	Herschel PACS and SPIRE observations of Galactic cold cores. Use of Planck data.
Ref:	=2010A&A...518L..93J
by	JUVELA M. , RISTORCELLI I., MONTIER L.A., MARSHALL D.J., PELKONEN V.-M., MALINEN J., YSARD N., TOTH L.V., HARJU J., BERNARD J.-P., SCHNEIDER N., VEREBELYI E., ANDERSON L., ANDRE P., GIARD M., KRAUSE O., LEHTINEN K., MACIAS-PEREZ J., MARTIN P., McGEHEE P.M., MENY C., MOTTE F., PAGANI L., PALADINI R., REACH W., VALENZIANO L., WARD-THOMPSON D., ZAVAGNO A.
	Astron. Astrophys., 518L, 93-93 (2010)
	Galactic cold cores: Herschel study of first planck detections.
o	Fig. 1, Table 2: <[JRM2010] PCC288-A> (Nos A-E), <[JRM2010] PCC550-PN> (Nos P1-P2), <[JRM2010] PCC249-PN> (Nos P1-P2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JRP2012]
[JRP2012]	(Juvela+Ristorcelli+Pagani+, 2012)
Write:	<<[JRP2012] JHHMMSS.s+DDMMSS>> <<[JRP2012] GLLL.ll+BB.bb filament>>
N:	53
Object:	Clump + Filament (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Herschel photometric observations of cold regions of the interstellar clouds as previously identified with the Planck satellite. N=102 clumps and N=26 filaments in 53 observed fields.
Ref:	=2012A&A...541A..12J
by	JUVELA M. , RISTORCELLI I., PAGANI L., DOI Y., PELKONEN V.-M., MARSHALL D.J., BERNARD J.-P., FALGARONE E., MALINEN J., MARTON G., McGEHEE P., MONTIER L.A., MOTTE F., PALADINI R., TOTH L.V., YSARD N., ZAHORECZ S., ZAVAGNO A.
	Astron. Astrophys., 541A, 12-12 (2012)
	Galactic cold cores. III. General cloud properties.
o	Table 2: <[JRP2012] JHHMMSS.s+DDMMSS> N=102. Table 3: <[JRP2012] GLLL.ll+BB.bb filament> N=26.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JRS2017]
[JRS2017]	(Jonsson+Ryde+Schultheis+, 2017)
Write:	<<[JRS2017] SW-NN>>
N:	11
Object:	* (SIMBAD class: Star)
Note:	VLT FLAMES UVES observations of N=11 stars in the Sagittarius Window in the galactic bulge. See also [LHZ2007].
Ref:	=2017A&A...598A.101J
by	JONSSON H. , RYDE N., SCHULTHEIS M., ZOCCALI M.
	Astron. Astrophys., 598A, 101-101 (2017)
	Abundances of disk and bulge giants from high-resolution optical spectra. II. O, Mg, Co, and Ti in the bulge sample.
o	(Erratum) erratum vol. 600, artc. C2 (2017)
o	Tables 1-2: <[JRS2017] SW-NN> N=11 among (Nos 09-76).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JRW2004]
[JRW2004]	(Jenkins+Roberts+Warwick+, 2004)= (XMM)
Write:	<<[JRW2004] XMM-NN>>
N:	14
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton observations of M 101. Use of Chandra data.
in source:	M 101
Ref:	=2004MNRAS.349..404J
by	JENKINS L.P. , ROBERTS T.P., WARWICK R.S., KILGARD R.E., WARD M.J.
	Mon. Not. R. Astron. Soc., 349, 404-424 (2004)
	An XMM-Newton view of M101 - I. The luminous X-ray source population.
o	Table 1: <[JRW2004] XMM-NN> (Nos 1-14).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JRW2005]
[JRW2005]	(Jenkins+Roberts+Ward+, 2005)= ([JRW2005a])
Write:	<<[JRW2005] NGC 7771 XN>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	XMM-Newton X-ray observations of the 2 interacting pairs. N=2 off-nuclear sources in NGC 7771.
in source:	NGC 7771
Ref:	=2005MNRAS.357..109J
by	JENKINS L.P. , ROBERTS T.P., WARD M.J., ZEZAS A.
	Mon. Not. R. Astron. Soc., 357, 109-123 (2005)
	XMM-Newton observations of the interacting galaxy pairs NGC 7771/0 and NGC 2342/1.
o	In Introduction, p.110 : NGC 4438/39 is a misprint for NGC 4038/39. In chap. 2.1, p.110 : Lyon Group of Galaxies numero 483 = LGG 483.
o	Fig.1, Table 1: <[JRW2005] NGC 7771 XN> (Nos X1-X2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JRW2005a]
[JRW2005a]	(Jenkins+Roberts+Ward+, 2005)
*****	Avoid the usage of [JRW2005a], prefer [JRW2005]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JRW2005b]
[JRW2005b]	(Jenkins+Roberts+Warwick+, 2005)
Write:	<<[JRW2005b] NNN>>
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton observations of M 101.
in source:	M 101 = NGC 5457
Ref:	=2005MNRAS.357..401J
by	JENKINS L.P. , ROBERTS T.P., WARWICK R.S., KILGARD R.E., WARD M.J.
	Mon. Not. R. Astron. Soc., 357, 401-419 (2005)
	An XMM-Newton view of M101 - II. Global X-ray source properties.
o	Table 1: <[JRW2005b] NNN> (Nos 1-108).
Ref:	=2007MNRAS.376.1611W
by	WARWICK R.S. , JENKINS L.P., READ A.M., ROBERTS T.P., OWEN R.A.
	Mon. Not. R. Astron. Soc., 376, 1611-1620 (2007)
	An XMM-Newton view of M101 - III. Diffuse X-ray emission.
o	Table A1: <[JRW2005b] NNN> (Nos 109-138) added.
=E=	Catalogue in electronic form as J/MNRAS/357/401
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSA2009]
[JSA2009]	(Johnston+Shepherd+Aguirre+, 2009)
Write:	<<[JSA2009] GLL.lll VLA NA>> <<[JSA2009] GLL.lll VLA NA-P>> <<[JSA2009] IRAS HHMMm+DDMM VLA NA>> <<[JSA2009] IRAS HHMMm+DDMM VLA NA-P>>
N:	70
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA 3.6cm (8.4GHz) observations of molecular clumps. In the format: if the observed field (Table 3, col.1) has two parts , eg. "G50.271 and G50.283", only the first part is kept in the format, eg. "G50.271 VLA 3A-P".
Ref:	=2009ApJ...707..283J
by	JOHNSTON K.G. , SHEPHERD D.S., AGUIRRE J.E., DUNHAM M.K., ROSOLOWSKY E., WOOD K.
	Astrophys. J., 707, 283-309 (2009)
	Ionized gas toward molecular clumps: physical properties of massive star-forming regions.
o	Tables 3, 5: <[JSA2009] GLL.lll VLA NA-P>, <[JSA2009] IRAS HHMMm+DDMM VLA NA-P> N=70.
=E=	Catalogue in electronic form as <J/ApJ/707/283/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSB2011]
[JSB2011]	(Jeffery+Smith+Brown+, 2011)
Write:	<<[JSB2011] NNNNN>>
N:	56
Object:	RR Lyr + Cepheid (SIMBAD class: Variable* = Variable Star)
Note:	HST ACS observations of RR Lyrae and Cepheids in six ultra-deep fields of M31, including part of the halo, disk and giant stellar stream.
in source:	M 31 = NGC 224
Ref:	=2011AJ....141..171J
by	JEFFERY E.J. , SMITH E., BROWN T.M., SWEIGART A.V., KALIRAI J.S., FERGUSON H.C., GUHATHAKURTA P., RENZINI A., RICH R.M.
	Astron. J., 141, 171 (2011)
	HST/ACS observations of RR Lyrae stars in six ultra-deep fields of M31.
o	Tables 3-8, 10-13: <[JSB2011] NNNNN> N=56 among (Nos 409-21631).
=E=	Catalogue in electronic form as J/AJ/141/171
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSB2014]
[JSB2014]	(Johnson+Sharon+Bayliss+, 2014)
Write:	<<[JSB2014] MACS J0416.0-2403 NN>> <<[JSB2014] MACS J0416.0-2403 NN.N>> <<[JSB2014] AS1063 NN>> <<[JSB2014] AS1063 NN.N>> <<[JSB2014] A370 N>> <<[JSB2014] A370 NN.N>>
N:	17+18+9+40+45+31
Object:	Grav. lensed image (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:	Magellan Baade telescope IMACS spectroscopy of N=17+18+9 systems of N=40+45+31 gravitationally lensed images in the field of three clusters of galaxies, as part of the Hubble Frontier Fields (HFF) initiative. Use of archival HST imaging data. See also [RJL2014] and [ZFM2015].
in source:	MCS J0416.1-2403
in source:	RXC J2248.7-4431 = ACO S 1063
in source:	ACO 370
Ref:	=2014ApJ...797...48J
by	JOHNSON T.L. , SHARON K., BAYLISS M.B., GLADDERS M.D., COE D., EBELING H.
	Astrophys. J., 797, 48 (2014)
	Lens models and magnification maps of the six Hubble frontier fields clusters.
o	There are differencies of identifications between Figure 6 and Table 11 (for example reversal between 2.3 and 2.5); the identifications fixed in SIMBAD are those of the table.
o	Table 7: <[JSB2014] MACS J0416.0-2403 NN> (Nos 1-17), <[JSB2014] MACS J0416.0-2403 NN.N> N=40. Table 10: <[JSB2014] AS1063 NN> (Nos 1-18), <[JSB2014] AS1063 NN.N> N=45. Table 11: <[JSB2014] A370 N> (Nos 1-9), <[JSB2014] A370 N.N> N=31.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSB2017]
[JSB2017]	(Jiang+Shen+Bian+, 2017)
Write:	<<[JSB2017] NN>>
N:	32
Object:	LAE (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	Magellan Clay M2FS spectroscopy of N=32 very luminous Lymanα emitters (LAEs). See also [NJZ2020], [NJZ2022].
in source:	NAME SXDSF
in source:	ACO 370
in source:	NAME ECDFS
in source:	NAME COSMOS Field
in source:	SSA 22
Ref:	=2017ApJ...846..134J
by	JIANG L. , SHEN Y., BIAN F., ZHENG Z.-Y., WU J., OYARZUN G.A., BLANC G.A., FAN X., HO L.C., INFANTE L., WANG R., WU X.-B., MATEO M., BAILEY J.I., CRANE J.D., OLSZEWSKI E.W., SHECTMAN S., THOMPSON I., WALKER M.G.
	Astrophys. J., 846, 134-134 (2017)
	A Magellan M2FS spectroscopic survey of galaxies at 5.5 < z < 6.8: program overview and a sample of the brightest Lyα emitters.
o	Figs 5+11, Table 4: <[JSB2017] NN> (Nos 1-32).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSD2005]
[JSD2005]	(Jimenez-Bailon+Santos-Lleo+Dahlem+, 2005) (Not yet in Simbad)
Write:	<<[JSD2005] SN>>
N:	2
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra ACIS observations of NGC 1808.
in source:	NGC 1808
Ref:	=2005A&A...442..861J
by	JIMENEZ-BAILON E. , SANTOS-LLEO M., DAHLEM M., EHLE M., MAS-HESSE J.M., GUAINAZZI M., HECKMAN T.M., WEAVER K.A.
	Astron. Astrophys., 442, 861-877 (2005)
	X-ray emission from NGC 1808: more than a complex starburst.
o	Fig.4, Table 2: <[JSD2005] SN> (Nos S1-S2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSD2012]
[JSD2012]	(Johnson+Seth+Dalcanton+, 2012)
Write:	<<[JSD2012] PC NNNN>> <<[JSD2012] NNN>>
N:	601+237+8+370
Object:	Cluster of * + Poss. Cluster of * + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST ACS and WFPC3 observations of M 31 as part of the Panchromatic Hubble Andromeda Treasury (PHAT) survey.
in source:	M 31
Ref:	=2012ApJ...752...95J
by	JOHNSON L.C. , SETH A.C., DALCANTON J.J., CALDWELL N., FOUESNEAU M., GOULIERMIS D.A., HODGE P.W., LARSEN S.S., OLSEN K.A.G., SAN ROMAN I., SARAJEDINI A., WEISZ D.R., WILLIAMS B.F., BEERMAN L.C., BIANCHI L., DOLPHIN A.E., GIRARDI L., GUHATHAKURTA P., KALIRAI J., LANG D., MONACHESI A., NANDA S., RIX H.-W., SKILLMAN E.D.
	Astrophys. J., 752, 95 (2012)
	PHAT stellar cluster survey. I. Year 1 catalog and integrated photometry.
o	Tables 1+2+8: <[JSD2012] PC NNNN> N=601+237+6 among (Nos 1-1728), Table 6: <[JSD2012] NNN> (Nos 1-370).
=E=	Catalogue in electronic form as <J/ApJ/752/95/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSD2015]
[JSD2015]	(Johnson+Seth+Dalcanton+, 2015)
Write:	<<[JSD2015] AP NNNNN>> <<[JSD2015] AAP NNNN>>
N:	2753+2270+8775+421+162+1430
Object:	Cluster of * + Poss. Cluster of * + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	A stellar cluster catalog for the Panchromatic Hubble Andromeda Treasury (PHAT) survey using image classifications collected from the Andromeda Project (AP) citizen science website. Andromeda Project (AP): we identify N=2753 clusters, N=2270 background galaxies, and N=8775 other candidates. Archival Andromeda Project (AAP): using additional, non-PHAT ACS images obtained from the HST archive, N=421 clusters, N=162 background galaxies, and N=1430 other candidates are identified. See also [JSD2012].
in source:	M 31 = NGC 224
Ref:	=2015ApJ...802..127J
by	JOHNSON L.C. , SETH A.C., DALCANTON J.J., WALLACE M.L., SIMPSON R.J., LINTOTT C.J., KAPADIA A., SKILLMAN E.D., CALDWELL N., FOUESNEAU M., WEISZ D.R., WILLIAMS B.F., BEERMAN L.C., GOULIERMIS D.A., SARAJEDINI A.
	Astrophys. J., 802, 127 (2015)
	PHAT stellar cluster survey. II. Andromeda project cluster catalog.
o	Tables 2+B1+C1: <[JSD2015] AP NNNNN> N=2753+2270+8775 among (Nos 1-54269). Tables E1-E3: <[JSD2015] AAP NNNN> N=421+162+1430 among (Nos 1-2041).
=E=	Catalogue in electronic form as <J/ApJ/802/127/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSE2010]
[JSE2010]	(Jones+Swinbank+Ellis+, 2010)
Write:	<<[JSE2010] Cl HHMM+DDMM>> <<[JSE2010] MACS JHHMM+DDMM>> <<[JSE2010] A>> <<[JSE2010] AN>>
N:	6+7
Object:	G + Grav. lensed image of a G (SIMBAD class: Galaxy)
Note:	Keck II OSIRIS observations of strongly lensed star-forming galaxies.
Ref:	=2010MNRAS.404.1247J
by	JONES T.A. , SWINBANK A.M., ELLIS R.S., RICHARD J., STARK D.P.
	Mon. Not. R. Astron. Soc., 404, 1247-1262 (2010)
	Resolved spectroscopy of gravitationally lensed galaxies: recovering coherent velocity fields in subluminous z ~ 2-3 galaxies.
o	Table 1: <[JSE2010] Cl HHMM+DDMM> N=2, <[JSE2010] MACS JHHMM+DDMM> N=4. Table 2: <[JSE2010] AN> (Nos A-D, E1-E2, F).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSE87]
[JSE87]	(Johnston+Simon+Eckart+, 1987)
Write:	<<[JSE87] 1928+738 N>>
N:	7
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	Components of QSO 1928+738 at 20cm wavelengths. See also [HSK92], [GMR98b], [GMP2000].
in source:	QSO B1928+738
Ref:	=1987ApJ...313L..85J
by	JOHNSTON K.J. , SIMON R.S., ECKART A., BIERMANN P., SCHALINSKI C., WITZEL A., STROM R.G.
	Astrophys. J., 313, 85-90 (1987)
	1928+738 : a superluminal source with large-scale structure.
o	Table 1, Fig.1: <[JSE87] 1928+738 N> (Nos 1-7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSF82]
[JSF82]	(Jaffe+Stier+Fazio, 1982)
Write:	<<[JSF82] FIR LLL.ll+B.bb>> <<[JSF82] Rad LLL.ll+B.bb>>
N:	42+32
Object:	(IR) + (Rad) (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 1: N=42 Far-IR sources, and N=32 radio continuum sources associated with the IR. See also [JGD81]
Ref:	=1982ApJ...252..601J
by	JAFFE D.T. , STIER M.T., FAZIO G.G.
	Astrophys. J., 252, 601-609 (1982)
	A high-resolution far-infrared survey of a section of the galactic plane. I. The nature of the sources.
o	Table 1: <[JSF82] FIR LLL.ll+B.bb> N=42, <[JSF82] Rad LLL.ll+B.bb> N=32
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSG2008]
[JSG2008]	(Johnston-Hollitt+Sato+Gill+, 2008)
Write:	<<[JSG2008] JHHMMSS.ss+DDMMSS.s>>
N:	52+36+22
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	ATCA 1.4GHz and 2.5GHz continuum observations of ACO 3158.
in source:	ACO 3158 = CA 0340-538
Ref:	=2008MNRAS.390..289J
by	JOHNSTON-HOLLITT M. , SATO M., GILL J.A., FLEENOR M.C., BRICK A.-M.
	Mon. Not. R. Astron. Soc., 390, 289-303 (2008)
	Radio observations of the Horologium-Reticulum supercluster - I. A3158: excess star-forming galaxies in a merging cluster ?
o	Tables 3, 4, 5: <[JSG2008] JHHMMSS.ss+DDMMSS.s> N=52+36+22.
=E=	Catalogue in electronic form as J/MNRAS/390/289
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSG2017]
[JSG2017]	(Johnson+Sharon+Gladders+, 2017)
Write:	<<[JSG2017] JHHMMSS.ss+DDMMSS.s>> <<[JSG2017] SDSS J1110+6459 A>> <<[JSG2017] SDSS J1110+6459 AN>> <<[JSG2017] SDSS J1110+6459 AaN>> <<[JSG2017] SDSS J1110+6459 AA>> <<[JSG2017] SDSS J1110+6459 NN>>
N:	27+39+24
Object:	G + Poss. Grav. lensed image + Clump (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST WFC3, Gemini North GMOS and MMT Blue Channel spectrograph observations of N=27 galaxies in the field of the galaxy cluster ClG J1110+6459, as well as N=38 grav. lensed images and image candidates, and N=24 clumps in the background source SGAS J111020.0+645950.
in source:	ClG J1110+6459
Ref:	=2017ApJ...843...78J
by	JOHNSON T.L. , SHARON K., GLADDERS M.D., RIGBY J.R., BAYLISS M.B., WUYTS E., WHITAKER K.E., FLORIAN M., MURRAY K.T.
	Astrophys. J., 843, 78-78 (2017)
	Star formation at z = 2.481 in the lensed galaxy SDSS J1110+6459. I. Lens modeling and source reconstruction.
o	Table 1: <[JSG2017] JHHMMSS.ss+DDMMSS.s> N=27. Fig. 3, Table 2: <[JSG2017] SDSS J1110+6459 A> (Nos A-F), <[JSG2017] SDSS J1110+6459 AN> N=22 among (Nos A1-A3 to F1-F3), <[JSG2017] SDSS J1110+6459 AaN> N=18 among (Nos Aa1-Aa3 to Ae1-Ae3), <[JSG2017] SDSS J1110+6459 AA> (Nos AX, AY). Fig. 9, Table 4: <[JSG2017] SDSS J1110+6459 NN> N=24 among (Nos 3-26).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSH2011]
[JSH2011]	(Johansson+Sigurdarson+Horellou, 2011)
Write:	<<[JSH2011] SMM JHHMMSS.s+DDMMSS>>
N:	37
Object:	smm G (SIMBAD class: Galaxy)
Note:	APEX LABOCA observations of N=37 submilliter galaxies behind five galaxy clusters.
Ref:	=2011A&A...527A.117J
by	JOHANSSON D. , SIGURDARSON H., HORELLOU C.
	Astron. Astrophys., 527A, 117-117 (2011)
	A LABOCA survey of submillimeter galaxies behind galaxy clusters.
o	Table 3: <[JSH2011] SMM JHHMMSS.s+DDMMSS> N=37.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSK2008]
[JSK2008]	(Jackson+Safi-Harb+Kothes+, 2008)
Write:	<<[JSK2008] SNR LL.l+B.b NN>>
N:	21+27
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton observations of the sources surrounding 2 SNRs.
Ref:	=2008ApJ...674..936J
by	JACKSON M.S. , SAFI-HARB S., KOTHES R., FOSTER T.
	Astrophys. J., 674, 936-953 (2008)
	XMM-Newton, Chandra, and CGPS observations of the supernova remnants G85.4+0.7 and G85.9-0.6.
o	Table 2, counterpart USNO-A2.0 1350-130274980 is a misprint for USNO-A2.0 1350-13027480. Table 3, counterpart 2MASS J20582367+4446195 is a misprint for 2MASS J20582387+4446195.
o	Table 2: <[JSK2008] SNR 85.4+0.7 NN> (Nos 1-21). Table 3: <[JSK2008] SNR 85.9+0.6 NN> (Nos 1-27).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSM2003]
[JSM2003]	(Jimenez-Bailon+Santos-Lleo+Mas-Hesse+, 2003)
Write:	<<[JSM2003] a>>
N:	17
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of NGC 4303. (Nos a-r) are point-like sources, (No. x) is an extended source. See also [THJ2000].
in source:	NGC 4303
Ref:	=2003ApJ...593..127J
by	JIMENEZ-BAILON E. , SANTOS-LLEO M., MAS-HESSE J.M., GUAINAZZI M., COLINA L., CERVINO M., GONZALEZ-DELGADO R.M.
	Astrophys. J., 593, 127-141 (2003)
	Nuclear activity and massive star formation in the low-luminosity active galactic nucleus NGC 4303: Chandra X-ray observations.
o	NGC 4559 X-1 = [VPB97] 1
o	Table 1, Fig.2: <[JSM2003] a> (Nos a-m, o-r, x).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSM2014]
[JSM2014]	(Jamrozy+Stawarz+Marchenko+, 2014)
Write:	<<[JSM2014] W>>
N:	2
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	VLA observations of N=2 cometary-like structures in the central region of ACO 585.
Ref:	=2014MNRAS.441.1260J
by	JAMROZY M. , STAWARZ L., MARCHENKO V., KUZMICZ A., OSTROWSKI M., CHEUNG C.C., SIKORA M.
	Mon. Not. R. Astron. Soc., 441, 1260-1269 (2014)
	Peculiar radio structures in the central regions of galaxy cluster Abell 585.
o	Paragr. 4.1: <[JSM2014] W> (Nos E, W).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Jsp
Jsp	(Discoverer's name: Jessup)= (Jessup)
Write:	<<** Jsp NNN>>
N:	803
Object:	(SIMBAD class: = Double or Multiple Star)
Ref:	=1955POMic..11....1R
by	ROSSITER R.A.
	Publ. Michigan Obs., 11, 1-None (1955)
	Catalogue of southern double stars.
o	Catalogue: < Don NNNN> N=1031 among (Nos 1-1057). < Jsp NNN> N=803 among (Nos 1-854). < RDS NNNN> (Nos 1-8065). < Rst NNNN> N=5534 among (Nos 1-5560).
Details on Acronym: [JSP95]
[JSP95]	(Jenness+Scott +Padman, 1995)= (FIR) = (SMM)
Write:	<<[JSP95] SMM HHMMSS.s+DDMMSS>> <<[JSP95] IRAS HHMMm+DDMM FIR N>>
N:	53
Object:	(Submm) (SIMBAD class: smmRad = Sub-Millimetric Source)
Note:	JCMT 450 and 850mu.m continuum observations of N=53 sub-millimeter sources associated with 42 IRAS sources. Among them, N=17 are also (FIR) sources.
Ref:	=1995MNRAS.276.1024J
by	JENNESS T. , SCOTT P.F., PADMAN R.
	Mon. Not. R. Astron. Soc., 276, 1024-1040 (1995)
	Studies of embedded far-infrared sources in the vicinity of H2O masers - I. Observations.
o	Table 2: HH 4 = GGD 4, HH 32-35 = NAME GGD 32-35.
o	Table 2, cols(2,3): <[JSP95] SMM HHMMSS.s+DDMMSS> N=53. Table 2, col(5): <[JSP95] IRAS HHMMm+DDMM FIR N> N=17.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSR2014]
[JSR2014]	(Jennings+Strader+Romanowsky+, 2013)
Write:	<<[JSR2014] ANNN>> <<[JSR2014] UCDNN>>
N:	781+31
Object:	Poss. GlCl + Poss. UCD (SIMBAD class: GlobCluster_Candidate = Globular Cluster Candidate)
Note:	HST ACS and Subaru SuprimeCam photometry of N=360+421 globular cluster candidates and N=31 ultra-compact dwarf candidates around NGC 3115.
in source:	NGC 3115
Ref:	=2014AJ....148...32J
by	JENNINGS Z.G. , STRADER J., ROMANOWSKY A.J., BRODIE J.P., ARNOLD J.A., LIN D., IRWIN J.A., SIVAKOFF G.R., WONG K.-W.
	Astron. J., 148, 32 (2014)
	The SLUGGS survey: HST/ACS mosaic imaging of the NGC 3115 globular cluster system.
o	Table 2: <[JSR2014] ANNN> (Nos A1-A360, S361-S781). Table 3: <[JSR2014] UCDNNN> (Nos UCD1-UCD31).
=E=	Catalogue in electronic form as <J/AJ/148/32/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSR2018]
[JSR2018]	(Jones+Scolnic+Riess+, 2018)
Write:	<<[JSR2018] pscNNNNNN>> <<[JSR2018] psYYMMNNN Host G>> <<[JSR2018] pscNNNNNN Host G>>
N:	1165+4+1165
Object:	SN + G (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=1165 supernovae and N=4+1165 host galaxies, using Pan-STARRS data.
Ref:	=2018ApJ...857...51J
by	JONES D.O. , SCOLNIC D.M., RIESS A.G., REST A., KIRSHNER R.P., BERGER E., KESSLER R., PAN Y.-C., FOLEY R.J., CHORNOCK R., ORTEGA C.A., CHALLIS P.J., BURGETT W.S., CHAMBERS K.C., DRAPER P.W., FLEWELLING H., HUBER M.E., KAISER N., KUDRITZKI R.-P., METCALFE N., TONRY J., WAINSCOAT R.J., WATERS C., GALL E.E.E., KOTAK R., McCRUM M., SMARTT S.J., SMITH K.W.
	Astrophys. J., 857, 51-51 (2018)
	Measuring dark energy properties with photometrically classified Pan-STARRS supernovae. II. Cosmological parameters.
o	Redshifts for host galaxies that have been put in SIMBAD are those given in table 2.
o	Table 2: <[JSR2018] pscNNNNNN> N=1165 among (Nos psc000006-psc590248). Table 3: <[JSR2018] psYYMMNNN Host G> N=4, <[JSR2018] pscNNNNNN Host G> N=1165.
=E=	Catalogue in electronic form as <J/ApJ/857/51/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSR2019]
[JSR2019]	(Jones+Sharp+Reiter+, 2019)
Write:	<<[JSR2019] Spitzer R>>
N:	3
Object:	Star Forming Region (SIMBAD class: StarFormingReg = Star Forming Region)
Note:	N=3 star formation regions in NGC 6822. Use of Spitzer data.
in source:	NGC 6822
Ref:	=2019MNRAS.490..832J
by	JONES O.C. , SHARP M.J., REITER M., HIRSCHAUER A.S., MEIXNER M., SRINIVASAN S.
	Mon. Not. R. Astron. Soc., 490, 832-847 (2019)
	The young stellar population of the metal-poor galaxy NGC 6822.
o	Fig. 10, Table 9: <[JSR2019] Spitzer R> (Nos I-III).
=E=	Catalogue in electronic form as <J/MNRAS/490/832/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JSW2022]
[JSW2022]	(Johnson+Schaye+Walth+, 2022) (Not yet in Simbad)
Write:	<<[JSW2022] GNN>> <<[JSW2022] NE nebula>> <<[JSW2022] S nebula>> <<[JSW2022] N ﬁlament>> <<[JSW2022] Host nebula>>
N:	27+1+1+1+1
Object:	G + Giant Nebula (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST COS and ACS, MUSE, Magellan LDSS3 observations of N=27 galaxies and N=4 nebulae in the field of TXS 0206-048.
Ref:	=2022ApJ...940L..40J
by	JOHNSON S.D. , SCHAYE J., WALTH G.L., LI J.I.-H., RUDIE G.C., CHEN H.-W., CHEN M.C., EPINAT B., GASPARI M., CANTALUPO S., KOLLATSCHNY W., LIU Z., MUZAHID S.
	Astrophys. J., 940L, 40 (2022)
	Directly Tracing Cool Filamentary Accretion over >100 kpc into the Interstellar Medium of a Quasar Host at z = 1.
o	Fig. 4, Table 1: <[JSW2022] GNN> (Nos G1-G27). Fig. 1, Table 2: <[JSW2022] NE nebula> N=1, <[JSW2022] S nebula> N=1, <[JSW2022] N filament> N=1, <[JSW2022] Host nebula> N=1.
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: [JT98]
[JT98]	(Jeffries+Tolley, 1998)
Write:	<<[JT98] NNNA>>
N:	102+49
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT HRI observations of NGC 2547. Search for optical counterparts of X-ray sources. N=102 X-ray sources, (Nos 1-102), some having several possible optical counterparts, numbered 'NNNA'.
in source:	NGC 2547
Ref:	=1998MNRAS.300..331J
by	JEFFRIES R.D. , TOLLEY A.J.
	Mon. Not. R. Astron. Soc., 300, 331-351 (1998)
	X-ray emission and low-mass stars in the young open cluster NGC 2547.
o	Tables 1, 2: <[JT98] NNN> (Nos 1-102), <[JT98] NNNA> N=49.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JTF2007]
[JTF2007]	(Jaunsen+Thoene+Fynbo+, 2007)
Write:	<<[JTF2007] Host Galaxy>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ESO VLT observations of GRB 070306.
Ref:	=2007GCN..6202....1J
by	JAUNSEN A.O. , THOENE C.C., FYNBO J.P.U., HJORTH J., VREESWIJK P.
	GCN, 6202, 1 (2007)
	GRB 070306: possible emission-line redshift.
o	<[JTF2007] Host Galaxy> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JTH2008]
[JTH2008]	(Jiang+Tamura+Hoare+, 2008) (Not yet in Simbad)
Write:	<<[JTH2008] IRAS 23033+5951 IRN N>> <<[JTH2008] IRAS 23033+5951 SN>>
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Note:	CIAO Subaru telescope observations of IRAS 23033+5951: N=3 IR Reflexion Nebulosity + N=1 pointlike source.
in source:	IRAS 23033+5951
Ref:	=2008ApJ...673L.175J
by	JIANG Z. , TAMURA M., HOARE M.G., YAO Y., ISHII M., FANG M., YANG J.
	Astrophys. J., 673L, 175-179 (2008)
	Disks around massive young stellar objects: are they common?
o	Fig.1d: <[JTH2008] IRAS 23033+5951 IRN N> (Nos 1-3), <[JTH2008] IRAS 23033+5951 SN> (No. S1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JTH2014]
[JTH2014]	(Jonker+Torres+Hynes+, 2014)= (GBS)
Write:	<<[JTH2014] CXBNNN>>
N:	424
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	N=424 X-ray sources from the Chandra Galactic Bulge Survey. See also CXOGBS.
Ref:	=2014ApJS..210...18J
by	JONKER P.G. , TORRES M.A.P., HYNES R.I., MACCARONE T.J., STEEGHS D., GREISS S., BRITT C.T., WU J., JOHNSON C.B., NELEMANS G., HEINKE C.
	Astrophys. J., Suppl. Ser., 210, 18 (2014)
	The Galactic Bulge Survey: completion of the X-ray survey observations.
o	Table 1, col(1): <CXOGBS JHHMMSS.s+DDMMSS> N=424 added, Table 1, col(2): <[JTH2014] CXBNNN> (Nos CXB1-CXB424).
=E=	Catalogue in electronic form as J/ApJS/210/18
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JTP
JTP	(Jeffries+Thurston+Pye)
*****	Avoid the usage of JTP, prefer JTX
Origin	of the Acronym: L (2004ApJ...606..466W)
Details on Acronym: JTS
JTS	(Jeffries+Thurston+, Source)
Write:	<<JTS N>>
N:	6
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations. Table 3: Soft-band sources, (Nos 1-6). See also JTX Table 2
in source:	NGC 2516
Ref:	=1997MNRAS.287..350J
by	JEFFRIES R.D. , THURSTON M.R., PYE J.P.
	Mon. Not. R. Astron. Soc., 287, 350-380 (1997)
	An X-ray survey of the young open cluster NGC 2516.
o	Table 2: <JTX NNN> (Nos 1-159). Table 3: <JTS N> (Nos 1-6).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [JTS98]
[JTS98]	(Jackson+Tadhunter+Sparks, 1998)
Write:	<<[JTS98] A>> <<[JTS98] N>>
N:	3+8
Object:	* + Region (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	Table 3: (Nos A-C), N=3 * near to Cyg A. Fig.5: (Nos 1-8), N=8 major blue condensations regions
Ref:	=1998MNRAS.301..131J
by	JACKSON N. , TADHUNTER C., SPARKS W.B.
	Mon. Not. R. Astron. Soc., 301, 131-141 (1998)
	Cygnus A : stars, dust and cones.
o	Table 3: <[JTS98] A> (Nos A-C). Fig.5: <[JTS98] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JTX
JTX	(Jeffries+Thurston+, X-ray source)= (JTP)
Write:	<<JTX NNN>>
N:	159
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations. Table 2: Hard-band sources, (Nos 1-159). See also JTS Table 3. See also paper II: [MSJ2000].
in source:	NGC 2516
Ref:	=1997MNRAS.287..350J
by	JEFFRIES R.D. , THURSTON M.R., PYE J.P.
	Mon. Not. R. Astron. Soc., 287, 350-380 (1997)
	An X-ray survey of the young open cluster NGC 2516.
o	Table 2: <JTX NNN> (Nos 1-159). Table 3: <JTS N> (Nos 1-6).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Ju
Ju	(Jurasovitch) (Not yet in Simbad)
Write:	<<Ju N>>
N:	1
Object:	PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Note:	Ju 1 = PN G075.5+01.7
Ref:	=2009CBET.1876....1J
by	JURASEVICH D.M.
	CBET, 1876, 1 (2009)
	PN G75.5+1.7.
o	<PN Ju N> (No. 1).
Details on Acronym: Juchert
Juchert	(Juchert)
Write:	<<Juchert NN>>
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Note:	From a private communication of Juchert. Some Juchert clusters are found in 2002A&A...389..871D and in 2006A&A...447..921K.
Auth.:	JUCHERT M.
=E=	Catalogue in electronic form as B/ocl
Origin	of the Acronym: L (2002A&A...389..871D)
Details on Acronym: [JV2005]
[JV2005]	(Janssen+Van Kerkwijk, 2005) (Not yet in Simbad)
Write:	<<[JV2005] NNNN>>
N:	2390
Object:	* (SIMBAD class: Star)
Note:	VLT observations of the field around PSR 1718-19.
Ref:	=2005A&A...439..433J
by	JANSSEN T. , VAN KERKWIJK M.H.
	Astron. Astrophys., 439, 433-441 (2005)
	Observations of the companion to the pulsar PSR B1718-19. The role of tidal circularisation.
o	Table 2: <[JV2005] NNNN> (Nos 1-2390).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JVAS
JVAS	(Jodrell-Bank VLA Astrometric Survey)= (PBWW)
Write:	<<JVAS HHMM+DD>> <<JVAS HHMM+DDd>> <<JVAS JHHMM+DDd>> <<JVAS JHHMM+DDMM>>
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Note:	The authors use the 2 formats 1950 and 2000 coordinates.
Ref:	=1992MNRAS.254..655P
by	PATNAIK A.R. , BROWNE I.W.A., WILKINSON P.N., WROBEL J.M.
	Mon. Not. R. Astron. Soc., 254, 655-None (1992)
	Interferometer phase calibration sources - I. The region 35° ≤ Dec. ≤ 75°.
o	<JVAS HHMM+DDd> = <JVAS JHHMM+DDd> N=858
Ref:	=1998MNRAS.293..257B
by	BROWNE I.W.A. , PATNAIK A.R., WILKINSON P.N., WROBEL J.M.
	Mon. Not. R. Astron. Soc., 293, 257-287 (1998)
	Interferometer phase calibration sources - II. The region 0° ≤ δ(B1950) ≤ +20°.
o	(Erratum) Correction in appendix B of paper III: 1998, MNRAS Vol. 300, p. 790.
o	<JVAS HHMM+DDd> = <JVAS JHHMM+DDMM> N=781.
Ref:	=1998MNRAS.300..790W
by	WILKINSON P.N. , BROWNE I.W.A., PATNAIK A.R., WROBEL J.M., SORATHIA B.
	Mon. Not. R. Astron. Soc., 300, 790-816 (1998)
	Interferometer phase calibrations sources - III. The regions +20° ≤ del_{B1950} ≤ +35° and +75° ≤ del_{B1950} ≤ +90° .
o	<JVAS HHMM+DDd> = <JVAS JHHMM+DDMM> N=540.
Ref:	=2002MNRAS.329..700S
by	SNELLEN I.A.G. , McMAHON R.G., HOOK I.M., BROWNE I.W.A.
	Mon. Not. R. Astron. Soc., 329, 700-746 (2002)
	Automated optical identification of a large complete northern hemisphere sample of flat-spectrum radio sources with S_{6cm}>200mJy.
o	Table A2: <JVAS JHHMM+DDMM> N=153.
=E=	Catalogue in electronic form as VIII/60
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [JVD2011]
[JVD2011]	(Jeffery+von Hippel+DeGennaro+, 2011)
Write:	<<[JVD2011] WDN>>
N:	7
Object:	Poss. WD (SIMBAD class: WhiteDwarf_Candidate = White Dwarf Candidate)
Stat:	is completely incorporated in Simbad
Note:	HST WFPC2 observations of N=7 cluster white dwarf candidates in NGC 2477.
in source:	NGC 2477
Ref:	=2011ApJ...730...35J
by	JEFFERY E.J. , VON HIPPEL T., DEGENNARO S., VAN DYK D.A., STEIN N., JEFFERYS W.H.
	Astrophys. J., 730, 35 (2011)
	The white dwarf age of NGC 2477.
o	Table 4: <[JVD2011] WDN> (Nos WD1-WD7).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JVH94]
[JVH94]	(Johnston+Verbunt+Hasinger)
Write:	<<[JVH94] NGC NNNN NNa>>
N:	123
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations of 8 Globular Clusters.
in source:	NGC 5139 = ome Cen
in source:	NGC 6341 = M 92
in source:	NGC 6397
in source:	NGC 6544
in source:	NGC 6626 = M 28
in source:	NGC 6656 = M 22
in source:	NGC 6752
in source:	NGC 7099 = M 30
Ref:	=1994A&A...289..763J
by	JOHNSTON H.M. , VERBUNT F., HASINGER G.
	Astron. Astrophys., 289, 763-774 (1994)
	ROSAT PSPC observations of globular clusters.
o	Tables 2-9: <[JVH94] NGC 5139 NN> (Nos 1-17), <[JVH94] NGC 6341 NN> (Nos 1-13), <[JVH94] NGC 6397 NN> (Nos 1-10), <[JVH94] NGC NGC 6544 N> (Nos 1-2), <[JVH94] NGC 6626 N> (Nos 1-4), <[JVH94] NGC 6656 N> (Nos 1-8), <[JVH94] NGC 6752 NN> (Nos 1-12), <[JVH94] NGC 7099 NN> (Nos 1-12).
Ref:	=2000A&A...358..910V
by	VERBUNT F. , JOHNSTON H.M.
	Astron. Astrophys., 358, 910-922 (2000)
	Multiple and variable X-ray sources in the globular clusters ω Cen, NGC 6397, NGC 6752, and Liller 1.
o	Table 2: <[JVH94] NGC 5139 NNa> (Nos 9a-9b, 18-21) added. Table 3: <[JVH94] NGC 6397 NNa> (Nos 4a-4e, 11-19) added. Table 6: <[JVH94] NGC 6752 NNa> (Nos 7a-7b, 13-22) added.
Ref:	=2001A&A...368..137V
by	VERBUNT F.
	Astron. Astrophys., 368, 137-159 (2001)
	A census with ROSAT of low-luminosity X-ray sources in globular clusters.
o	Table 2: see also [FLM96], [HCJ97], [HG83b], [HGB93], [JVH94], [JVH96], [RDL94].
o	Table 2: <[V2001] NGC NNNN XNNa> N=49, <[V2001] JHHMMSS.ss+DDMMSS.s> N=2, <[FLM96] M 13 Aa> (Nos F, Ga-Gb, R-T) added, <[HCJ97] NN> (Nos 6-10) added, <[HGB93] A> (No. G) added, <[JVH94] NGC 6626 NNa> (Nos 5-12, 2a-2c) added, <[JVH94] NGC 6656 N> (No. 9) added, <[JVH94] NGC 7099 NN> (No. 13) added, <[JVH96] NGC 6121 NN> (Nos 7-10) added, <[JVH96] NGC 6352 NN> (No. 17) added, <[JVH96] NGC 6366 NN> (Nos 7-8) added.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JVH95]
[JVH95]	(Johnston+Verbunt+Hasinger, 1995)
Write:	<<[JVH95] Terzan 5 S2>>
N:	1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT observations of Cl Terzan 5 have revealed two sources XB 1745-25 and a second source designated as S2.
in source:	Cl Terzan 5
Ref:	=1995A&A...298L..21J
by	JOHNSTON H.M. , VERBUNT F., HASINGER G.
	Astron. Astrophys., 298, 21-24 (1995)
	The positions of the X-ray sources in the globular clusters Terzan 1, Terzan 5 and NGC 6440.
o	PSR M15C = PSR 2127+11C, MX 1746-20 = 1M 1746-203
o	Table 2: <[JVH95] Terzan 5 SN> (No. S2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JVH96]
[JVH96]	(Johnston+Verbunt+Hasinger, 1996)
Write:	<<[JVH96] NGC NNNN NN>>
N:	115
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT PSPC observations of 10 globular clusters.
in source:	NGC 3201
in source:	NGC 4372
in source:	NGC 6121 = M 4
in source:	NGC 6254 = M 10
in source:	NGC 6352
in source:	NGC 6366
in source:	NGC 6496
in source:	NGC 6652
in source:	NGC 6760
in source:	NGC 6809 = M 55
Ref:	=1996A&A...309..116J
by	JOHNSTON H.M. , VERBUNT F., HASINGER G.
	Astron. Astrophys., 309, 116-122 (1996)
	ROSAT observations of ten globular clusters with large core radii.
o	Table 2: <[JVH96] NNNN NN> N=109.
Ref:	=2001A&A...368..137V
by	VERBUNT F.
	Astron. Astrophys., 368, 137-159 (2001)
	A census with ROSAT of low-luminosity X-ray sources in globular clusters.
o	Table 2: see also [FLM96], [HCJ97], [HG83b], [HGB93], [JVH94], [JVH96], [RDL94].
o	Table 2: <[V2001] NGC NNNN XNNa> N=49, <[V2001] JHHMMSS.ss+DDMMSS.s> N=2, <[FLM96] M 13 Aa> (Nos F, Ga-Gb, R-T) added, <[HCJ97] NN> (Nos 6-10) added, <[HGB93] A> (No. G) added, <[JVH94] NGC 6626 NNa> (Nos 5-12, 2a-2c) added, <[JVH94] NGC 6656 N> (No. 9) added, <[JVH94] NGC 7099 NN> (No. 13) added, <[JVH96] NGC 6121 NN> (Nos 7-10) added, <[JVH96] NGC 6352 NN> (No. 17) added, <[JVH96] NGC 6366 NN> (Nos 7-8) added.
=E=	Catalogue in electronic form as J/A+A/309/116
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JVL99]
[JVL99]	(Johnson+Vacca+Leitherer+, 1999)
Write:	<<[JVL99] NNN>>
N:	434
Object:	Super star Cl (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	HST FOC, WFPC2 GHRS observations of NGC 1741.
in source:	NGC 1741
Ref:	=1999AJ....117.1708J
by	JOHNSON K.E. , VACCA W.D., LEITHERER C., CONTI P.S., LIPSCY S.J.
	Astron. J., 117, 1708-1724 (1999)
	The very young starburst merger system NGC 1741.
o	Table 2: <[JVL99] NNN> (Nos 1-434).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JVW2005]
[JVW2005]	(Jarvis+Van Breukelen+Wilman, 2005)
Write:	<<[JVW2005] JHHMM+DDMM>>
N:	2
Object:	QSO (SIMBAD class: QSO = Quasar)
Stat:	is completely incorporated in Simbad
Note:	Serendipitous discovery of QSOs from VIMOS on the VLT.
Ref:	=2005MNRAS.358L..11J
by	JARVIS M.J. , VAN BREUKELEN C., WILMAN R.J.
	Mon. Not. R. Astron. Soc., 358, 11-15 (2005)
	The discovery of a type II quasar at z= 1.65 with integral-field spectroscopy.
o	CXO 52 is CXOU J084837.9+445352, Object CDF-S 202 = [GZW2002] XID 202 = CXOCDFS J033229.9-275106
o	Text: <[JVW2005] JHHMM+DDMM> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JW
JW	(Jones+Walker)
Write:	<<JW NNNN>>
N:	1053
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Stars within 15 arcmin of the center of the Orion nebula. See also [H97b] were (Nos 1-1053) are identical to JW NNNN.
in source:	NAME Orion Nebula
Ref:	=1988AJ.....95.1755J
by	JONES B.F. , WALKER M.F.
	Astron. J., 95, 1755-1782 (1988)
	Proper motions and variabilities of stars near the Orion Nebula.
o	Finding charts
o	Table III: <JW NNNN> (Nos 1-1053).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [JW2016]
[JW2016]	(Jithesh+Wang, 2015)
Write:	<<[JW2016] TNN>>
N:	15
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton observations of N=15 transient X-ray sources in NGC 55. See also [SRW2006].
in source:	NGC 55
Ref:	=2016ApJ...821...24J
by	JITHESH V. , WANG Z.
	Astrophys. J., 821, 24-24 (2016)
	Transient X-ray source population in the magellanic-type galaxy NGC 55.
o	Table 2: <[JW2016] TNN> (Nos T1-T15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JWB2005]
[JWB2005]	(Jones+Woodward+Boyer+, 2005)
Write:	<<[JWB2005] NNN>> <<[JWB2005] NNN.N>> <<[JWB2005] JHHMMSS+DDMMSS>> <<[JWB2005] JHHMMSS.ss+DDMMSS.s>>
N:	48+1+2
Object:	(IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	IRAC on the Spitzer Space Telescope observations of LHA 120-N 159 in the LMC. N=48 sources selected from the entire point-source data, and 2 point-like added with only coordinates 'JHHMMSS.ss+DDMMSS.s'. A radio peak is also observed at 'J053953-694518'.
in source:	Magellanic Clouds:LMC:LHA 120-N 159 = LHA 120-N 159
Ref:	=2005ApJ...620..731J
by	JONES T.J. , WOODWARD C.E., BOYER M.L., GEHRZ R.D., POLOMSKI E.
	Astrophys. J., 620, 731-743 (2005)
	Spitzer IRAC observations of star formation in N159 in the Large Magellanic Cloud.
o	Tables 1, 2: <[JWB2005] NNN.N> N=48. Text: <[JWB2005] JHHMMSS+DDMMSS> N=1, <[JWB2005] JHHMMSS.ss+DDMMSS.s> N=2.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JWB2017]
[JWB2017]	(Jordan+Walsh+Breen+, 2021)
Write:	<<[JWB2017] GLLL.ll+BB.bb>> <<[JWB2017] GLLL.lll+BB.bbb>>
N:	4+74
Object:	CH3OH Maser (SIMBAD class: Maser)
Stat:	is completely incorporated in Simbad
Note:	N=4+74 CH3OH masers, as part of the MALT45 (Millimetre Astronomer’s Legacy Team-45 GHz) Galactic Plane survey, using the Australia Telescope Compact Array. See also [JWL2015].
Ref:	=2017MNRAS.471.3915J
by	JORDAN C.H. , WALSH A.J., BREEN S.L., ELLINGSEN S.P., VORONKOV M.A., HYLAND L.J.
	Mon. Not. R. Astron. Soc., 471, 3915-3954 (2017)
	MALT-45: A 7 mm survey of the southern Galaxy - II. ATCA follow-up observations of 44 GHz class I methanol masers.
o	Table 2, col(1): <[JWB2017] GLLL.ll+BB.bb> (Nos G331.44-00.14, G331.44-00.16, G333.01-00.46, G333.12-0.43). Table 2, col(2): <[JWB2017] GLLL.lll+BB.bbb> N=74.
=E=	Catalogue in electronic form as <J/MNRAS/471/3915/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JWB2018]
[JWB2018]	(Jiang+Wu+Bian+, 2019)
Write:	<<[JWB2018] SXDS gPC>> <<[JWB2018] LAE NN>>
N:	1+46
Object:	Protocluster + LAE (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Magellan Clay telescope M2FS observations of N=1 giant protocluster and N=46 Lyman Alpha Emitters (LAEs) in the Subaru XMM-Newton Deep Survey (SXDS) field.
in source:	NAME SXDF
Ref:	=2018NatAs...2..962J
by	JIANG L. , WU J., BIAN F., CHIANG Y.-K., HO L.C., SHEN Y., ZHENG Z.-Y., BAILEY III J.I., BLANC G.A., CRANE J.D., FAN X., MATEO M., OLSZEWSKI E.W., OYARZUN G.A., WANG R., WU X.-B.
	NatAs, 2, 962-966 (2018)
	A giant protocluster of galaxies at redshift 5.7.
o	<[JWB2018] SXDS gPC> N=1. Suppl. Table 1: <[JWB2018] LAE NN> (Nos 1-46).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
History	of this Acronym: replaces [JWB2019]
Details on Acronym: [JWF2005]
[JWF2005]	(Jee+White+Ford+, 2005)
Write:	<<[JWF2005] MN>>
N:	4
Object:	Clump (SIMBAD class: Gravitation = Gravitational Source)
Stat:	is completely incorporated in Simbad
Note:	HST ACS weak lensing analysis of 1E 1054.4-0321 = ClG 1054-03. N=3 mass peaks were first identified by [HFK2000]. N=4 minor peaks are identified: (Nos M1-M4).
in source:	1E 1054.4-0321 = ClG 1054-0321
Ref:	=2005ApJ...634..813J
by	JEE M.J. , WHITE R.L., FORD H.C., BLAKESLEE J.P., ILLINGWORTH G.D., COE D.A., TRAN K.-V.H.
	Astrophys. J., 634, 813-832 (2005)
	Hubble Space Telescope Advanced Camera for Surveys weak-lensing and Chandra X-ray studies of the high-redshift cluster MS 1054-0321.
o	Table 1: objects W, C, E are [HFK2000] W, C, E in SIMBAD.
o	Fig.16, Table 1: <[JWF2005] MN> (Nos M1-M4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JWG2003]
[JWG2003]	(Jackson+Werner+Gautier, 2003) (Not yet in Simbad)
Write:	<<[JWG2003] NNN>>
N:	141
Object:	Filament (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	List of the prominent filamentary structures in the interstellar cirrus.
Ref:	=2003ApJS..149..365J
by	JACKSON T. , WERNER M., GAUTIER III T.N.
	Astrophys. J., Suppl. Ser., 149, 365-373 (2003)
	A catalog of bright filamentary structures in the interstellar medium.
o	Tables 1, 2, 3: <[JWG2003] NNN> (Nos 1-141).
=E=	Catalogue in electronic form as J/ApJS/149/365
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JWK2004]
[JWK2004]	(Jones+Woodward+Kelley, 2004)
Write:	<<[JWK2004] G192.16-3.84 Star N>> <<[JWK2004] G192.16-3.84 RfN N>> <<[JWK2004] W42 Star NN>> <<[JWK2004] W42 RfN N>> <<[JWK2004] Cep A Star N>>
N:	8+8+16+5+5
Object:	* + RfN (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Near-IR polarimetry at the NASA IRTF 3m telescope of three regions of massive star formation.
in source:	GAL 192.16-03.84
in source:	W 42
in source:	NAME Cep A
Ref:	=2004AJ....128.2448J
by	JONES T.J. , WOODWARD C.E., KELLEY M.S.
	Astron. J., 128, 2448-2459 (2004)
	Outflows from luminous young stellar objects: an infrared polarimetric study.
o	Table 2: <[JWK2004] G192.16-3.84 Star N> (Nos 1-8). Table 3: <[JWK2004] G192.16-3.84 RfN N> (Nos 1-8). Table 4: <[JWK2004] W42 Star NN> (Nos 1-16). Table 5: <[JWK2004] W42 RfN N> (Nos 1-5). Table 6: <[JWK2004] Cep A Star N> (Nos 1-5).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JWL2015]
[JWL2015]	(Jordan+Walsh+Lowe+, 2015)
Write:	<<[JWL2015] GLLL.ll+BB.bb>>
N:	77+47
Object:	CH3OH Maser + SiO Maser (SIMBAD class: Maser)
Note:	N=77+47 CH3OH and SiO masers respectively, as part of the MALT45 (Millimetre Astronomer’s Legacy Team-45 GHz) Galactic Plane survey, using the Australia Telescope Compact Array. See also [JWB2017].
Ref:	=2015MNRAS.448.2344J
by	JORDAN C.H. , WALSH A.J., LOWE V., VORONKOV M.A., ELLINGSEN S.P., BREEN S.L., PURCELL C.R., BARNES P.J., BURTON M.G., CUNNINGHAM M.R., HILL T., JACKSON J.M., LONGMORE S.N., PERETTO N., URQUHART J.S.
	Mon. Not. R. Astron. Soc., 448, 2344-2361 (2015)
	MALT-45: a 7 mm survey of the southern Galaxy - I. Techniques and spectral line data.
o	Tables 2-3: <[JWL2015] GLLL.ll+BB.bb> N=77+47.
=E=	Catalogue in electronic form as <J/MNRAS/448/2344/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JWM2000]
[JWM2000]	(Johnstone+Wilson+Moriarty-Schieven+, 2000)= (SMM)
Write:	<<[JWM2000] SMM JHHMMm-DDMMa>>
N:	55
Object:	Clump (SIMBAD class: PartofCloud = Part of Cloud)
Note:	SCUBA observations on JCMT.
in source:	NAME rho Oph Cloud
Ref:	=2000ApJ...545..327J
by	JOHNSTONE D. , WILSON C.D., MORIARTY-SCHIEVEN G., JONCAS G., SMITH G., GREGERSEN E., FICH M.
	Astrophys. J., 545, 327-339 (2000)
	Large-area mapping at 850 microns. II. Analysis of the clump distribution in the ρ Ophiuchi molecular cloud.
o	in ref list Maddox et al 1990MNRAS.242p.43 instead of 242.43
o	Table 1: <[JWM2000] SMM JHHMMm-DDMMa> N=55.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JWM2012]
[JWM2012]	(Jennings+Williams+Murphy+, 2012)= (BW)
Write:	<<[JWM2012] BW-NNN>>
N:	27+13
Object:	SNR (SIMBAD class: SNRemnant = SuperNova Remnant)
Note:	SNRs with Deep 2-Filter HST Data in M31.
in source:	M 31
Ref:	=2012ApJ...761...26J
by	JENNINGS Z.G. , WILLIAMS B.F., MURPHY J.W., DALCANTON J.J., GILBERT K.M., DOLPHIN A.E., FOUESNEAU M., WEISZ D.R.
	Astrophys. J., 761, 26 (2012)
	Supernova remnant progenitor masses in M31.
o	Table 1: <[JWM2012] BW-NNN> N=27 among (Nos 11-110).
Ref:	=2014ApJ...795..170J
by	JENNINGS Z.G. , WILLIAMS B.F., MURPHY J.W., DALCANTON J.J., GILBERT K.M., DOLPHIN A.E., WEISZ D.R., FOUESNEAU M.
	Astrophys. J., 795, 170 (2014)
	The supernova progenitor mass distributions of M31 and M33: further evidence for an upper mass limit.
o	Table 1: <[JWM2012] BW-NNN> N=13 among (Nos 45-101).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JWP2006]
[JWP2006]	(Jorgenson+Wolfe+Prochaska+, 2006)
Write:	<<[JWP2006] QSO JHHMM+DDMM abs N.NNNN>>
N:	8
Object:	DLA
Stat:	is completely incorporated in Simbad
Note:	Spectroscopic observations at the 200inch telescope at Palomar Observatory. Search for DLAs in radio-selected QSOs.
Ref:	=2006ApJ...646..730J
by	JORGENSON R.A. , WOLFE A.M., PROCHASKA J.X., LU L., HOWK J.C., COOKE J., GAWISER E., GELINO D.M.
	Astrophys. J., 646, 730-741 (2006)
	The UCSD radio-selected quasar survey for damped Lyα systems.
o	Table 2: <[JWP2006] QSO JHHMM+DDMM abs N.NNNN> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: JWT
JWT	(Jessop+Ward-Thompson)
Write:	<<JWT Cloud FFFA>> <<JWT Core NN>>
N:	16+60
Object:	Cloud + Part of Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	Table 1: N=16 clouds. In the format, 'FFF' stands for the ISSA (IRAS Sky Survey Atlas) field number. Table 2: N=60 molecular clouds in the 16 clouds.
Ref:	=2000MNRAS.311...63J
by	JESSOP N.E. , WARD-THOMPSON D.
	Mon. Not. R. Astron. Soc., 311, 63-74 (2000)
	A far-infrared survey of molecular cloud cores.
o	Table 1: <JWT Cloud FFFA> N=16. Table 2: <JWT Core NN> (Nos 1-60).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [JWW2013]
[JWW2013]	(Johnson+Wilson+Wang+, 2013)
Write:	<<[JWW2013] JHHMMSS.ss+DDMMSS.s>>
N:	45
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of N=45 AzTEC sources in the GOODS-North, GOODS-South and COSMOS fields.
in source:	NAME GOODS North Field
in source:	NAME GOODS South Field
in source:	NAME COSMOS Field
Ref:	=2013MNRAS.431..662J
by	JOHNSON S.P. , WILSON G.W., WANG Q.D., WILLIAMS C.C., SCOTT K.S., YUN M.S., POPE A., LOWENTHAL J., ARETXAGA I., HUGHES D., KIM M.J., KIM S., TAMURA Y., KOHNO K., EZAWA H., KAWABE R., OSHIMA T.
	Mon. Not. R. Astron. Soc., 431, 662-682 (2013)
	X-ray detections of submillimetre galaxies: active galactic nuclei versus starburst contribution.
o	Tables 1-2: <[JWW2013] JHHMMSS.ss+DDMMSS.s> N=45.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: 1Jy
1Jy	(1Jy (flux density))= (J)
Write:	<<1Jy HHMM+DD>> <<1Jy HHMM+DDd>>
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1981A&AS...45..367K
by	KUHR H. , WITZEL A., PAULINY-TOTH I.I.K., NAUBER U.
	Astron. Astrophys., Suppl. Ser., 45, 367-430 (1981)
	A catalogue of extragalactic radio sources having flux densities greater than 1Jy at 5 GHz.
o	reprint in the special issue (500/1) : 2009A&A...500..215K
o	Table III: <1Jy HHMM+DD>, <1Jy HHMM+DDd>, N=518
Ref:	=1994A&AS..105..211S
by	STICKEL M. , MEISENHEIMER K., KUEHR H.
	Astron. Astrophys., Suppl. Ser., 105, 211-234 (1994)
	The optical identification status of the 1 Jy radio source catalogue.
o	<1Jy HHMM+DDd> N=527
=E=	Catalogue in electronic form as VIII/5
=E=	Catalogue in electronic form as J/A+AS/105/211
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [JYI97]
[JYI97]	(Jannuzi+Yanny+Impey, 1997)
Write:	<<[JYI97] MS HHMM.m+DDMM A>>
N:	3+20+15
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	HST WFPC-2 observations. Objects in the field of 3 BL Lac MS objects (1E 1221.8+2452, 1E 1407.9+5954, 1E 2143.4+0704). Maps in Plates 3-5
Ref:	=1997ApJ...491..146J
by	JANNUZI B.T. , YANNY B., IMPEY C.
	Astrophys. J., 491, 146-152 (1997)
	Hubble Space Telescope imaging of the host galaxies of three x-ray-selected BL Lacertae objects.
o	no coordinates, objects not in SIMBAD
o	Table 1: <[JYI97] MS 1221.8+2452 A> (Nos A-C). Table 2: <[JYI97] MS 1407.9+5954 A> (Nos A-T). Table 3: <[JYI97] MS 2143.4+0704 A> (Nos A-O).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JYY2001]
[JYY2001]	(Jiang+Yao+Yang+, 2001) (Not yet in Simbad)
Write:	<<[JYY2001] S187IR Knot A>> <<[JYY2001] S233A Knot W>> <<[JYY2001] S233B Knot A>>
N:	9+4+4
Object:	Knot (SIMBAD class: Unknown = Object of Unknown Nature)
in source:	SH 2-187
in source:	SH 2-233
Ref:	=2001AJ....122..313J
by	JIANG Z. , YAO Y., YANG J., ISHII M., NAGATA T., NAKAYA H., SATO S.
	Astron. J., 122, 313-321 (2001)
	K'-band polarimetric imaging of S187 IR and S233.
o	Table 2 read IRAS 20188+3928 instead of IRAS 20188+2720. Fig.3: (Nos 1-22) from Yao+, not published, objects are not in SIMBAD.
o	Table 1, Fig2: <[JYY2001] S187IR Knot A> (Nos A-I), <[JYY2001] S233A Knot W> (Nos E, S, W, N), <JYY2001] S233B Knot A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JYY2002]
[JYY2002]	(Jiang+Yao+Yang+, 2002) (Not yet in Simbad)
Write:	<<[JYY2002] Region NW>> <<[JYY2002] Pillar N>> <<[JYY2002] Arc N>> <<[JYY2002] Triple N>> <<[JYY2002] KW object N>> <<[JYY2002] Brace N>>
N:	4+3+5+3+3+1
Object:	* (SIMBAD class: Star)
Note:	N=4 regions in M 17 complex. Stars in differents selected areas.
in source:	M 17 = NGC 6618
Ref:	=2002ApJ...577..245J
by	JIANG Z. , YAO Y., YANG J., ANDO M., KATO D., KAWAI T., KURITA M., NAGATA T., NAGAYAMA T., NAKAJIMA Y., NAGASHIMA C., SATO S., TAMURA M., NAKAYA H., SUGITANI K.
	Astrophys. J., 577, 245-259 (2002)
	Deep near-infrared survey toward the M17 region.
o	Table 3, Fig.3: <[JYY2002] Pillar N> (Nos 1-3), <[JYY2002] Arc N> (Nos 1-5), <[JYY2002] Triple N> (Nos 1-3), <[JYY2002] KW object N> (Nos 1-3), <[JYY2002] Brace N> (No. 1).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JYY2003]
[JYY2003]	(Jiang+Yao+Yang+, 2003)
Write:	<<[JYY2003] NIR NNN>> <<[JYY2003] H2 N>>
Object:	(Near IR) + H2 (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Observations from the IRSF telescope of Nagoya university at SAAO. Near-IR study of the region of Sh 2-269. N=367 sources associated with the Sh 2-269 nebula. N=6 H2 emssion features.
in source:	SH 2-269
Ref:	=2003ApJ...596.1064J
by	JIANG Z. , YAO Y., YANG J., BABA D., KATO D., KURITA M., NAGASHIMA C., NAGATA T., NAGAYAMA T., NAKAJIMA Y., ISHII M., TAMURA M., SUGITANI K.
	Astrophys. J., 596, 1064-1079 (2003)
	A near-infrared study of the star-forming region S269.
o	Table 1: <[JYY2003] NIR NNN> (Nos 1-367). Table 2: <[JYY2003] H2 N> (Nos 1-6).
=E=	Catalogue in electronic form as J/ApJ/596/1064
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JYY2004]
[JYY2004]	(Jiang+Yang+Yao+, 2004)
Write:	<<[JYY2004] N>>
N:	8
Object:	H2 (SIMBAD class: PartofCloud = Part of Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=8 H2 emission knots in the IRAS 20231+3440 region, observed with the Japanese Okayama 1.8m optical/near-infrared telescope.
Ref:	=2004ChA&A..28..299J
by	JIANG Z.-B. , YANG J., YAO Y.-Q., ISHI M., MAO R.-Q.
	Chinese Astron., 28, 299-307 (2004)
	Properties of the exciting source of the outflow in IRAS 20231+3440 region.
o	Fig.3, Table 1: <[JYY2004] N> (Nos 1-8).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JZB2004]
[JZB2004]	(Jaeger+Ziegler+Bohm+, 2004)
Write:	<<[JZB2004] MS 1008-12 ANNa>> <<[JZB2004] Cl 0303+17 ANNa>> <<[JZB2004] Cl 0413-65 ANNa>>
N:	38+2+38+4+38+5
Object:	G (SIMBAD class: Galaxy)
Note:	VLT FORS observations of galaxies in the regions of 3 distant galaxy clusters. Finding charts in Fig.3.
in source:	1E 1008.1-1224 = ClG 1008-1224
in source:	ClG 0303+1706
in source:	ClG 0413-6559
Ref:	=2004A&A...422..907J
by	JAEGER K. , ZIEGLER B.L., BOEHM A., HEIDT J., MOELLENHOFF C., HOPP U., MENDEZ R.H., WAGNER S.
	Astron. Astrophys., 422, 907-913 (2004)
	Internal kinematics of spiral galaxies in distant clusters. II. Observations and data analysis.
o	Table 2: <[JZB2004] MS 1008-12 ANNa> (Nos A1-A19, B1-B19, B7b, B8b). Table 3: <[JZB2004] Cl 0303+17 ANNa> (Nos A1-A19, B1-B19, A4b, A4c, A14b, A17b). Table 4: <[JZB2004] Cl 0413-65 ANNa> (Nos A1-A19, B1-B19, A9b, A12b, A17b, B8b, B10b).
=E=	Catalogue in electronic form as J/A+A/422/907
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JZH95]
[JZH95]	(Junkes+Zinnecker+Hensler+, 1995)
Write:	<<[JZH95] NNa>>
N:	21
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations.
in source:	NGC 1808
Ref:	=1995A&A...294....8J
by	JUNKES N. , ZINNECKER H., HENSLER G., DAHLEM M., PIETSCH W.
	Astron. Astrophys., 294, 8-22 (1995)
	NGC 1808: X-ray emission from the nuclear starburst.
o	Table 7: <[JZH95] NNa> (Nos 1-19), N=21
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [JZM2020]
[JZM2020]	(Jimenez-Andrade+Zavala+Magnelli+, 2020)
Write:	<<[JZM2020] AzTEC2-A>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	ALMA Band 7 and NOEMA Band 1 observations of N=2 components of the submillimeter galaxy AzTEC 2.
Ref:	=2020ApJ...890..171J
by	JIMENEZ-ANDRADE E.F. , ZAVALA J.A., MAGNELLI B., CASEY C.M., LIU D., ROMANO-DIAZ E., SCHINNERER E., HARRINGTON K., ARETXAGA I., KARIM A., STAGUHN J., BURNHAM A.D., MONTANA A., SMOLCIC V., YUN M., BERTOLDI F., HUGHES D.
	Astrophys. J., 890, 171-171 (2020)
	The redshift and star formation mode of AzTEC2: a pair of massive galaxies at z = 4.63.
o	Fig. 1, Table 1: <[JZM2020] AzTEC2-A> (Nos AzTEC2-A, AzTEC2-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: K
K	(Konkoly obs.) (Not yet in Simbad)
Write:	<<K NN>>
N:	7
Object:	Flare * (SIMBAD class: Eruptive* = Eruptive Variable)
Note:	Szecsenyi-Nagy
Details on Acronym: K
K	(Klemola) (Not yet in Simbad)
*****	Avoid the usage of K, prefer [K62]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: K
K	(Kunchev+) (Not yet in Simbad)
*****	Avoid the usage of K, prefer [KK97]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: K
K	(Kuz'min) (Not yet in Simbad)
*****	Avoid the usage of K, prefer KLNS
Details on Acronym: K
K	(Karpov)
Write:	<<** K N>>
N:	4
Object:	(SIMBAD class: = Double or Multiple Star)
Stat:	is completely incorporated in Simbad
Note:	Table II
Ref:	=1937PASP...49..146K
by	KARPOV B.G.
	Publ. Astron. Soc. Pac., 49, 146-147 (1937)
	Proper motions larger than 0".20 found in four northern Bruce regions.
o	Table I: <[K37] 1-NN> (Nos 1-36). Table II: <** K N> (Nos 1-4)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: K
K	(King)
*****	Avoid the usage of K, prefer King
Details on Acronym: K
K	(Kron)
*****	Avoid the usage of K, prefer Kron
Details on Acronym: K
K	(Kukarkin)
*****	Avoid the usage of K, prefer CSV
Details on Acronym: K
K	(Kerr)
*****	Avoid the usage of K, prefer [H68]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: K
K	(Karpov)
*****	Avoid the usage of K, prefer [K37]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: K
K	(Khavtasi)
*****	Avoid the usage of K, prefer [K55]
Details on Acronym: K
K	(Khavtasi)
*****	Avoid the usage of K, prefer [K60]
Details on Acronym: K
K	(Karachentseva)
*****	Avoid the usage of K, prefer K68
Origin	of the Acronym: L = Found in the literature
Details on Acronym: K
K	(Kron)
*****	Avoid the usage of K, prefer [K80]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: K
K	(Kinman+)
*****	Avoid the usage of K, prefer [KGM79]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: K
K	(Kelly+)
*****	Avoid the usage of K, prefer KK
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: K
K	(Kontizas+)
*****	Avoid the usage of K, prefer KMHK
Origin	of the Acronym: L (1997AJ....114.1002Z)
Details on Acronym: K
K	(Karachentsev)
*****	Avoid the usage of K, prefer KPG
Origin	of the Acronym: L = Found in the literature
Details on Acronym: K
K	(Kiso obs.)
*****	Avoid the usage of K, prefer KUV
Origin	of the Acronym: L (1986AJ.....91..139W)
Details on Acronym: K
K	(Krautter+)
*****	Avoid the usage of K, prefer [KWS97]
Origin	of the Acronym: L (1998A&A...330..521W)
Details on Acronym: K
K	(Kohoutek)
Write:	<<PN K 1-NN>> <<PN K 2-NN>> <<PN K 3-NN>> <<PN K 4-NN>> <<PN K 5-NN>> <<PN K 6-NN>>
N:	33+17+94+60+39+42
Object:	PN + Poss. PN (SIMBAD class: PlanetaryNeb = Planetary Nebula)
Stat:	is completely incorporated in Simbad
Ref:	=1962BAICz..13..120K
by	KOHOUTEK L.
	Bull. Astron. Inst. Czech., 13, 120-None (1962)
	New planetary nebulae.
o	<PN K 1-N> (Nos 1-1 to 1-6).
Ref:	=1963BAICz..14...70K
by	KOHOUTEK L.
	Bull. Astron. Inst. Czech., 14, 70-74 (1963)
	New planetary nebulae.
o	Table 1: <PN K 1-NN> (Nos 1-7 to 1-20). Table 2: <PN K 2-N> (Nos 2-1 to 2-7).
Ref:	=1964BAICz..15..162K
by	KOHOUTEK L.
	Bull. Astron. Inst. Czech., 15, 162-None (1964)
	New planetary nebulae.
o	<PN K 2-NN> (Nos 2-8 to 2-11).
Ref:	=1971A&A....13..493K
by	KOHOUTEK L.
	Astron. Astrophys., 13, 493-495 (1971)
	New planetary nebulae.
o	Table 1: <PN K 1-NN> (Nos 1-21 to 1-25). Table 2: <PN K 2-NN> (Nos 2-12 to 2-15).
Ref:	=1977A&A....59..137K
by	KOHOUTEK L.
	Astron. Astrophys., 59, 137-139 (1977)
	New southern planetary nebulae.
o	<PN K 1-NN> (Nos 1-26 to 1-33), <PN K 2-NN> (Nos 2-16 to 2-17)
Ref:	=1965BAICz..16..221K
by	KOHOUTEK L.
	Bull. Astron. Inst. Czech., 16, 221-227 (1965)
	Hamburg Schmidt-camera survey of faint planetary nebulae.
o	Table 3: <PN K 3-NN> (Nos 3-1 to 3-63). Table 4: <PN K 4-NN> (Nos 4-1 to 4-46)
Ref:	=1969BAICz..20..307K
by	KOHOUTEK L.
	Bull. Astron. Inst. Czech., 20, 307-382 (1969)
	Hamburg Schmidt-camera survey of faint planetary nebulae.
o	Table 2: <PN K 3-NN> (Nos 3-64 to 3-72). Table 3: <PN K 4-NN> (Nos 4-47 to 4-50). Table 5: <Kohoutek N> (Nos 1-5).
Ref:	=1972A&A....16..291K
by	KOHOUTEK L.
	Astron. Astrophys., 16, 291-300 (1972)
	Hamburg Schmidt camera survey of faint planetary nebulae. Cygnus-Perseus region.
o	Table 2: <PN K 3-NN> (Nos 3-73 to 3-94). Table 3: <PN K 4-NN> (Nos 4-51 to 4-60). Table 5: <Kohoutek N> (Nos 6, 7a-7c, 8).
Ref:	=1994AN....315..235K
by	KOHOUTEK L.
	Astron. Nachr., 315, 235-244 (1994)
	New planetary nebulae towards the galactic bulge. I. Objects in the central area.
o	PK 3+2 2 not IRAS 17414-2412, cross-id Te 5 uncorrect, Te 1567, 1580, 2111 not in SIMBAD
o	Table 3: <PN K 5-NN> (Nos 5-1 to 5-20). Table 4: <PN K 6-NN> (Nos 6-1 to 6-17)
Ref:	=2002AN....323...57K
by	KOHOUTEK L.
	Astron. Nachr., 323, 57-70 (2002)
	New planetary nebulae towards the Galactic Bulge. II. Objects surrounding the central area.
o	Table 3: <PN K 5-NN> (Nos 5-21 to 5-39). Table 4: <PN K 6-NN> (Nos 6-18 to 6-42).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: K
K	(Kitt Peak obs.)
*****	Avoid the usage of K, prefer SKHB
Origin	of the Acronym: L = Found in the literature
Details on Acronym: K
K	(Knot)
*****	Avoid the usage of K, prefer [WB92a]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: K17
K17	(Kerzendorf, 2017)
Write:	<<K17 A>> <<K17 -A>> (not recognised by Simbad, but found in literature)
N:	4
Object:	Poss. * (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=4 star candidates near Cas A. Use of HST ACS/WFC and WFC3-IR archival data.
Ref:	=2019A&A...623A..34K
by	KERZENDORF W.E. , DO T., DE MINK S.E., GOTBERG Y., MILISAVLJEVIC D., ZAPARTAS E., RENZO M., JUSTHAM S., PODSIADLOWSKI P., FESEN R.A.
	Astron. Astrophys., 623A, 34-34 (2019)
	No surviving non-compact stellar companion to Cassiopeia A.
o	Figs 3-4, Tables 2-3: <K17 A> (Nos W-Z).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: K2
K2	(Kepler Extended Mission)
Write:	<<K2 -NNN>>
Object:	* (SIMBAD class: Star)
Note:	As part of the Kepler extended mission, confirmed planets with K2 data receive a K2 designation K2-NN b. In the literature, the EPIC host is often assigned a K2 designation (without the lower-case letter). The list of K2 names is available here: http://exoplanetarchive.ipac.caltech.edu/cgi-bin/TblView/nph-tblView?app=ExoTbls&config=k2names
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: K2
K2	(Kepler Extended Mission)
Write:	<<K2 -NNNa>>
Object:	Planet (SIMBAD class: Planet = Extra-solar Planet)
Note:	As part of the Kepler extended mission, confirmed planets with K2 data receive a K2 designation K2-NN b. In the literature, the EPIC host is often assigned a K2 designation (without the lower-case letter). The list of K2 names is available here: http://exoplanetarchive.ipac.caltech.edu/cgi-bin/TblView/nph-tblView?app=ExoTbls&config=k2names
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: K20
K20	(K < 20 Survey)
*****	Avoid the usage of K20, prefer [DCR2004]
Origin	of the Acronym: L (2008ApJ...682..231S)
Details on Acronym: K20
K20	(K < 20 Survey)
*****	Avoid the usage of K20, prefer K20S
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [K2001]
[K2001]	(Kaaret, 2001)= ([K2001a])
Write:	<<[K2001] CN>>
N:	6
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra X-ray point sources in M 100. In the format the letter 'C' stands for Chandra.
in source:	M 100 = NGC 4321
Ref:	=2001ApJ...560..715K
by	KAARET P.
	Astrophys. J., 560, 715-718 (2001)
	Chandra X-ray point sources, including supernova 1979C, in the spiral galaxy M100.
o	Table 2: <[K2001] AN> (Nos C1-C6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K2001a]
[K2001a]	(Kaaret, 2001)
*****	Avoid the usage of [K2001a], prefer [K2001]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K2001b]
[K2001b]	(Komossa, 2001) (Not yet in Simbad)
Write:	<<[K2001b] XNN>>
N:	26
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	ROSAT PSPC observations of the field of MRC 2251-178.
Ref:	=2001A&A...367..801K
by	KOMOSSA S.
	Astron. Astrophys., 367, 801-808 (2001)
	The X-ray view of the quasar MR 2251-178 and its host cluster: Variability, absorption, and intracluster gas emission.
o	Figs 1, 2, Table 1: <[K2001b] XNN> N=25 among 36.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K2001c]
[K2001c]	(Kohler, 2001)
Write:	<<[K2001c] NN>> <<[K2001c] RX J1243.1-7458A>>
N:	82+3
Object:	TT* (SIMBAD class: TTauri* = T Tauri Star)
Note:	Search for multiplicity of a sample of X-ray selected young stars in Chamaeleon.
in source:	NAME Cha Region
Ref:	=2001AJ....122.3325K
by	KOEHLER R.
	Astron. J., 122, 3325-3334 (2001)
	Multiplicity of x-ray-selected T Tauri stars in Chamaeleon.
o	Tables 1, 2: <[K2001c] NN> (Nos 1-82). Table 1: <[K2001c] RX J1243.1-7458A> (Nos A-C).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K2002]
[K2002]	(Kaaret, 2002)
Write:	<<[K2002] JHHMMSS.ss+DDMMSS.s>>
N:	143
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	Chandra HRC observations of M 31. See also CXOM31 and [KGP2002].
in source:	M 31 = NGC 224
Ref:	=2002ApJ...578..114K
by	KAARET P.
	Astrophys. J., 578, 114-125 (2002)
	A Chandra high resolution camera observation of X-ray point sources in M31.
o	T.1: sources are also CXOM31 JHHMMSS.s+DDMMSS sources.
o	Table 1: <[K2002] JHHMMSS.ss+DDMMSS.s> N=143.
=E=	Catalogue in electronic form as J/ApJ/578/114
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K2003]
[K2003]	(Kurtev, 2003)= ([K2003a])
Write:	<<[K2003] JHHMMSS.ss+DDMMSS.s>>
N:	8
Object:	Poss. Blue Supergiant (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Observations from Mexican National Astronomical Observatory and Bulgarian National Astronomical Observatory. N=8 blue supergiant candidates in M 31.
in source:	M 31 = NGC 224
Ref:	=2003AN....324..265K
by	KURTEV R.G.
	Astron. Nachr., 324, 265-270 (2003)
	UBV and vby stellar photometry in the eastern part of M31.
o	OB 31-35 = [V64] 31 to 35 in SIMBAD.
o	Table 2: <[K2003] JHHMMSS.ss+DDMMSS.s> N=8.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K2003a]
[K2003a]	(Kurtev, 2003)
*****	Avoid the usage of [K2003a], prefer [K2003]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K2003b]
[K2003b]	(Khanzadyan, 2003) (Not yet in Simbad)
Write:	<<[K2003b] CB 3 a>>
N:	5
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	N=5 new H2 excited objects in [CB88] 3.
in source:	[CB88] 3
Ref:	=2003CoKon.103...31K
by	KHANZADYAN T.
	Comm. Konkoly Obs., 103, 31-36 (2003)
	Near-infrared study of large Bok globules.
o	Fig.2: Objects 'AN' in [CB88] 34 are [KSG2002] AN in SIMBAD. Fig.3: VLA 1, 2 = [YMT96] CB 39 1, 2.
o	Fig.1: <[K2003b] CB 3 a> (Nos a-e).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K2003c]
[K2003c]	(Kong, 2003)
Write:	<<[K2003c] XNN>>
N:	37
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	XMM-Newton observation of IC 342.
in source:	IC 342
Ref:	=2003MNRAS.346..265K
by	KONG A.K.H.
	Mon. Not. R. Astron. Soc., 346, 265-272 (2003)
	XMM-Newton observation of the X-ray point source population of the starburst galaxy IC 342.
o	Table 1: <[K2003c] XNN> (Nos X1-X37).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K2003d]
[K2003d]	(Khanzadyan, 2003)
Write:	<<[K2003d] rho Oph ANN>>
N:	7+11+3+2
Object:	H2 Knot (SIMBAD class: PartofCloud = Part of Cloud)
Note:	New H2 knots in Rho Oph cloud, from Khanzadyan PhD Thesis in 2003. Somme objects are found in 2004A&A...426..171K (see [KGS2004])
in source:	NAME rho Oph Cloud
Auth.:	KHANZADYAN T.+
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K2004a]
[K2004a]	(Keller, 2004)
Write:	<<[K2004] aaN-NN>>
N:	51
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Measurements of the projected rotational velocities of early B-type stars in the LMC fields (fp1 to fp4) and clusters.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=2004PASA...21..310K
by	KELLER S.C.
	Publications - Astron. Soc. Australia, 21, 310-317 (2004)
	Rotation of early B-type stars in the Large Magellanic Cloud : the role of evolution and metallicity.
o	Table 1: Cl* NGC 2004 ROB ANN, Cl* NGC 1818 ROB ANN.
o	Table 2: <[K2004a] fpN-NN> N=14+14+13+10.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K2004b]
[K2004b]	(Keel, 2004)
Write:	<<[K2004b] JHHMMSS.ss+DDMMSS.s>>
N:	1
Object:	G (SIMBAD class: Galaxy)
Note:	HST STIS and WYIN maps of the pair NGC 1409-NGC 1410. A fainter third galaxy is seen just east of NGC 1410.
Ref:	=2004AJ....127.1325K
by	KEEL W.C.
	Astron. J., 127, 1325-1335 (2004)
	Ongoing mass transfer in the interacting galaxy pair NGC 1409/1410.
o	object cited on p.1328: <[K2004b] JHHMMSS.ss+DDMMSS.s> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K2005]
[K2005]	(Kaaret, 2005)
Write:	<<[K2005] NN>> <<[K2005] Star A>>
N:	13+2
Object:	(X) + * (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	HST observations of NGC 1073.
in source:	NGC 1073
Ref:	=2005ApJ...629..233K
by	KAARET P.
	Astrophys. J., 629, 233-238 (2005)
	Optical sources near the bright X-ray source in NGC 1073.
o	Parag. 3 : Source X7 in NGC 4559 = [VPB97] 7
o	Table 1: <[K2005] NN> (Nos 1-13). Table 2: <[K2005] Star A> (Nos A-B).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K2010]
[K2010]	(Kent, 2010)
Write:	<<[K2010] {Cloud} N {North\|South\|West}>>
N:	5
Object:	HI Cloud (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	VLA observations of N=5 HI clouds as part of the ALFALFA survey.
in source:	[KGH2007] 1
in source:	[KGH2007] 2
Ref:	=2010ApJ...725.2333K
by	KENT B.R.
	Astrophys. J., 725, 2333-2343 (2010)
	Clouds toward the Virgo cluster periphery: gas-rich optically inert galaxies.
o	Figs 4-5, Table 4: <[K2010] Cloud N North> (Nos 1-2), <[K2010] Cloud N South> (Nos 1-2), <[K2010] Cloud 2 West> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K2019]
[K2019]	(Kong, 2019) (Not yet in Simbad)
Write:	<<[K2019] NNN>>
N:	280
Object:	Dense Core (SIMBAD class: denseCore = Dense Core)
Note:	ALMA 1.3 mm continuum observations of N = 280 cores in the infrared dark cloud G28.37+0.07.
in source:	NAME Dragon Nebula
Ref:	=2019ApJ...873...31K
by	KONG S.
	Astrophys. J., 873, 31-31 (2019)
	The core mass function in the infrared dark cloud G28.37+0.07.
o	Text: <[K2019] NNN> (Nos 1 to 280).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K20]
[K20]	(Knox-Shaw, 1920)= (KS)
Write:	<<[K20] NN>> <<[K20] A>>
N:	27+3
Object:	* (SIMBAD class: Star)
Note:	Stars in the field of NGC 6729. Tables I, III: N=27 among (Nos 1-70), N=3 (Nos R-S-T). Map in Plate I. Helwan Observatory, Bull. No. 20.
in source:	NGC 6729
Auth.:	KNOX-SHAW H.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: K20S
K20S	(K < 20 Survey)= (CDFS) = (K20)
Write:	<<K20S 0055-269 NNNN>> <<K20S CDFS NNNN>>
N:	198+348
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	K20 survey at the ESO VLT and NTT in two fields, CDFS and a field centered on QSO 0055-269. The first paper is the Ks photometric catalogue.
in source:	NAME CDFS
Ref:	=2002A&A...392..395C
by	CIMATTI A. , MIGNOLI M., DADDI E., POZZETTI L., FONTANA A., SARACCO P., POLI F., RENZINI A., ZAMORANI G., BROADHURST T., CRISTIANI S., D'ODORICO S., GIALLONGO E., GILMOZZI R., MENCI N.
	Astron. Astrophys., 392, 395-406 (2002)
	The K20 survey. III. Photometric and spectroscopic properties of the sample.
o	Catalog: <K20S 0055-269 NNNN> N=198, <K20S CDFS NNNN> N=348.
=E=	Catalogue in electronic form as J/A+A/392/395
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K37]
[K37]	(Karpov, 1937)
Write:	<<[K37] 1-NN>> <<[K37] 2-NN>> <<[K37] 3-NN>>
N:	36+46+12
Object:	PM* (SIMBAD class: HighPM* = High Proper Motion Star)
Note:	1937PASP...49..146K, Table I: 1st list, format '1-NN' (Nos 1-36). 1937AJ.....46..201K, Table I: 2nd list, format '2-NN' (Nos 1-46). 1937AJ.....46..201K, Table II: 3rd list, format '3-NN' (Nos 1-12)
Ref:	=1937PASP...49..146K
by	KARPOV B.G.
	Publ. Astron. Soc. Pac., 49, 146-147 (1937)
	Proper motions larger than 0".20 found in four northern Bruce regions.
o	Table I: <[K37] 1-NN> (Nos 1-36). Table II: <** K N> (Nos 1-4)
Ref:	=1937AJ.....46..201K
by	KARPOV B.G.
	Astron. J., 46, 201-203 (1937)
	Proper motions larger than 0".20 found in six northern Bruce regions.
o	Table I: <[K37] 2-NN> (Nos 1-46), Table II: <[K37] 3-NN> (Nos 1-12)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K55]
[K55]	(Khavtasi, 1955)= (K) = (Kh) = (Khav) = (Khavtasi) = (Khavtassi)
Write:	<<[K55] NNN>>
N:	797
Object:	Dark Nebula (SIMBAD class: DarkNeb = Dark Cloud (nebula))
Note:	Catalog. Different running numbers in the Catalog [K55] and in the Atlas [K60].
Ref:	=1955AbaOB..18...29K
by	KHAVTASI D.S.
	Byull. Abastumanskaya Astrofiz. Obs., 18, 29-114 (1955)
	A statistical study of dark nebulae (catalogue).
o	<[K55] NNN> (Nos 1-797)
Details on Acronym: [K60]
[K60]	(Khavtasi, 1960)= (K) = (Kh) = (Khav) = (Khavtasi) = (Khavtassi)
Write:	<<[K60] NNN>>
N:	762
Object:	Dark Nebula (SIMBAD class: DarkNeb = Dark Cloud (nebula))
Note:	Different running numbers in the Catalog [K55] and in the Atlas [K60].
Ref:	=1960AGDN..C......0K
by	KHAVTASI D.S.
	Byull. Abastumansk. Astrofiz. Obs. (in Russian), 0-None (1960)
	Atlas of galactic dark nebulae.
o	<[K60] NNN> (Nos 1-762).
Details on Acronym: [K62]
[K62]	(Klemola, 1962)= (K) = (Klemola) (Not yet in Simbad)
Write:	<<[K62] NNN>>
N:	205
Object:	Blue * (SIMBAD class: Star)
Ref:	=1962AJ.....67..740K
by	KLEMOLA A.R.
	Astron. J., 67, 740-756 (1962)
	Mean absolute magnitude of the blue stars at high galactic latitude.
o	Table I: <[K62] NNN> (Nos 1-205)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K67]
[K67]	(Kayser, 1967)
Write:	<<[K67] R>> <<[K67] ANNN>> <<[K67] VNN>>
N:	22+43+32
Object:	* (SIMBAD class: Star)
Note:	Table I: primary standards, (Nos I-XXII). Table II and text: N=43 * format 'ANNN' where the letter 'A' stands for fields (Nos A-G). p. 143-144: V* format 'VNN', (Nos V1-V32), (Nos V1-V15) being identical to [H25] VNN (Nos V1-V15) (Brian Skiff, 1999). See also [H25].
in source:	NGC 6822
Ref:	=1967AJ.....72..134K
by	KAYSER S.E.
	Astron. J., 72, 134-148 (1967)
	Photometry of the nearby irregular galaxy NGC 6822.
o	Table I: <[K67] R> (Nos I-XXII), Table II and text: <[K67] ANNN> N=43, p. 143-144: <[K67] VNN> (Nos V1-V32)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: K68
K68	(Karachentseva, 1968)= (K) = ([K68a]) = (Kar) = (Kara) = (Kara 68) = (Karachentseva) = KDG = (KDwG)
Write:	<<K68 NNN>> <<K68 NA>>
N:	241+8+4
Object:	Dwarf G (SIMBAD class: Galaxy)
Note:	(Nos 1-241) and (Nos 1N-8N). K68 1N to K68 8N = BK 1N to BK 8N. Later, 2 galaxies have been found as double: 224A and 224B, 232A and 232B.
Ref:	=1968SoByu..39...61K
by	KARACHENTSEVA V.E.
	Soobshch. Byurakan Obs., 39, 61-73 (1968)
	The distribution of Sculptor-type dwarf galaxies.
o	<K68 NNN> (Nos 1-241)
Ref:	=1998A&AS..127..397V
by	VAN DRIEL W. , KRAAN-KORTEWEG R.C., BINGGELI B., HUCHTMEIER W.K.
	Astron. Astrophys., Suppl. Ser., 127, 397-408 (1998)
	An HI line search for optically identified dwarf galaxy candidates in the M 81 group.
o	Table 1, col.1: <[B93] NN> (Nos 1-41), No. 5 missing. Table 1, col.2: <[VKB98] Anon N> (Nos 1-7). Table 1, col.2: <K68 NNNW> (Nos 1N-8N).
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [K68a]
[K68a]	(Karachentseva, 1968)
*****	Avoid the usage of [K68a], prefer K68
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K68b]
[K68b]	(Kinman, 1968)
Write:	<<[K68b] 3C 120 N>>
N:	4
Object:	* (SIMBAD class: Star)
Note:	Stars in the field of 3C 120
Ref:	=1968AJ.....73..885K
by	KINMAN T.D.
	Astron. J., 73, 885-887 (1968)
	Photographic photometry of the Seyfert galaxy 3C 120.
o	Plate S-VIII: <[K68b] 3C 120 N> (Nos 1-4).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K69]
[K69]	(Kohoutek, 1969)
Write:	<<[K69] a>>
N:	13
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	N=13 stars in the field of SV* HBV 475. Finding chart.
Ref:	=1969IBVS..384....1K
by	KOHOUTEK L.
	IAU Inform. Bull. Var. Stars, 384, 1-2 (1969)
	HBV 475: a new peculiar emission object in Cygnus.
o	Table 1: <[K69] a> (Nos a-m).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K70]
[K70]	(Kawajiri, 1970)= (NK) (Not yet in Simbad)
Write:	<<[K70] 1-NN>> <<[K70] 2-NN>>
N:	58+59
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Ref:	=1970PASJ...22..165K
by	KAWAJIRI N.
	Publ. Astron. Soc. Jap., 22, 165-175 (1970)
	Two continuum surveys along the galactic plane at 8000 MHz.
o	Table 2: <[K70] 1-NN> (Nos 1-1 to 1-58). Table 3: <[K70] 2-NN> (Nos 1-1 to 1-59).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: K72
K72	(Karachentsev, 1972)
====>	Equivalent to: KPG
Origin	of the Acronym: L = Found in the literature
Details on Acronym: K72
K72	(Karachentsev, 1972)
====>	Equivalent to: KPG
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [K72b]
[K72b]	(Karachentseva, 1972)
Write:	<<[K72b] NN>>
N:	20
Object:	Dwarf G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Ref:	=1972ATsir.723....1K
by	KARACHENTSEVA V.E.
	Astron. Tsirk., 723, 1-2 (1972)
	The Sculptor-type dwarf galaxies detected in the zone δ -30 of the Palomar Sky syrvey.
o	<[K72b] NN> (Nos 1-20)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K72c]
[K72c]	(Karlsson, 1972) (Not yet in Simbad)
Write:	<<[K72c] NNN>>
Object:	* (SIMBAD class: Star)
Note:	N=825 stars in a Monoceros field.
Ref:	=1972A&AS....7...35K
by	KARLSSON R.
	Astron. Astrophys., Suppl. Ser., 7, 35-81 (1972)
	The distribution of stars and obscuring matter in a Monoceros field.
o	Catalogue: <[K72c] NNN> (Nos 1-825).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: K73
K73	(Karachentseva, 1973)= (CIG) = (IG) = (Kar) = (Kara) = (KIG)
Write:	<<K73 NNNN>>
N:	1051
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	New positions in 2003A&A...411..391L.
Ref:	=1973SoSAO...8....3K
by	KARACHENTSEVA V.E.
	Soobshch. Spets. Astrof. Obs., 8, 3-72 (1973)
	The catalogue of isolated galaxies.
o	<K73 NNNN> (Nos 1-1051)
=E=	Catalogue in electronic form as VII/82
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [K76]
[K76]	(Kronberg, 1976)
Write:	<<[K76] 3C 303W>> <<[K76] 3C 303 A>>
N:	2+8
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	N=2 components of 3C 303, often designated as 3C 303E (eastern) and 3C 303W (western) in the literature. N=8 optical objects in the immediate vicinity of 3C 303, (Nos A-H). Warning: [K76] 3C 30E (eastern component of 3C 303) and [K76] 3C 303 E (E nearby optical object) are different objects in SIMBAD.
in source:	3C 303
Ref:	=1976ApJ...203L..47K
by	KRONBERG P.P.
	Astrophys. J., 203, 47-48 (1976)
	3C 303: A source with unusual radio and optical properties.
o	Warning: [K76] 3C 303E (eastern component of 3C 303) and [K76] 3C 303 E (E nearby optical object) are different objects in SIMBAD.
o	Text: <[K76] 3C 303W> (Nos E, W). Fig.2: <[K76] 3C 303 A> (Nos A-H).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K77]
[K77]	(Knude, 1977)
Write:	<<[K77] NNN>>
N:	756
Object:	* (SIMBAD class: Star)
Ref:	=1977A&AS...30..297K
by	KNUDE J.K.
	Astron. Astrophys., Suppl. Ser., 30, 297-305 (1977)
	Photoelectric uvby and H β photometry of 750 A and F stars in 63 selected areas with \|b\|<30.
o	Table 1: <[K77] NNN> N=756 among (Nos 22-868)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: K79
K79	(Karachentseva, 1979)= (KTG) = (T)
Write:	<<K79 NN>>
N:	84
Object:	Triplet of G (SIMBAD class: GroupG = Group of Galaxies)
Note:	Finding charts.
Ref:	=1979AISAO..11....3K
by	KARACHENTSEVA V.E. , KARACHENTSEV I.D., SHCHERBANOVSKY A.L.
	Astrofizik. Issledovanija, 11, 3-39 (1979)
	Isolated triplet of galaxies.
o	<K79 NN> (Nos 1-84), <K79 NNA> N=84x3
=E=	Catalogue in electronic form as VII/83
Origin	of the Acronym: L = Found in the literature
Details on Acronym: K79
K79	(Karachentseva, 1979)
Write:	<<K79 NNA>>
N:	84x3
Object:	G in triplet (SIMBAD class: GtowardsGroup = Galaxy towards a Group of Galaxies)
Note:	Finding charts.
Ref:	=1979AISAO..11....3K
by	KARACHENTSEVA V.E. , KARACHENTSEV I.D., SHCHERBANOVSKY A.L.
	Astrofizik. Issledovanija, 11, 3-39 (1979)
	Isolated triplet of galaxies.
o	<K79 NN> (Nos 1-84), <K79 NNA> N=84x3
=E=	Catalogue in electronic form as VII/83
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [K80]
[K80]	(Kron, 1980)= ([BHK94]) = (K) = ([K80a]) = ([KBW94]) = (Kron) = (NSer)
Write:	<<[K80] SA 57 NNNNN>> <<[K80] SA 68 NNNNN>> <<[K80] Herc-1 NNNNN>> <<[K80] Lynx-2 NNNNN>>
N:	about 20000
Object:	G (SIMBAD class: Galaxy)
Note:	1980ApJS...43..305K: description of the techniques, The complete list of objects in each of the 4 fields has not been published. Each field has is own numbering. See also [MKK97]: SA 57: NSer [MKK97] = NSer [K80] + 100000, SA 68: NSer [MKK97] = NSer [K80] + 200000.
Ref:	=1980ApJS...43..305K
by	KRON R.G.
	Astrophys. J., Suppl. Ser., 43, 305-325 (1980)
	Photometry of a complete sample of faint galaxies.
o	<[K80] SA 57 NNNNN>, <[K80] SA 68 NNNNN>, N about 20000
Ref:	=1986ApJ...311..651K
by	KOO D.C.
	Astrophys. J., 311, 651-679 (1986)
	Multicolor photometry of field galaxies to B 24.
o	Description of [K80] catalogues for SA 57 and SA 68
o	<[K80] SA 57 NNNNN>, <[K80] SA 68 NNNNN>.
Ref:	=1994AJ....108..870B
by	BERSHADY M.A. , HERELD M., KRON R.G., KOO D.C., MUNN J.A., MAJEWSKI S.R.
	Astron. J., 108, 870-895 (1994)
	The optical and near-infrared colors of galaxies. I. The photometric data.
o	Table 6: <[K80] SA 57 NNNNN>, <[K80] SA 68 NNNNN>, <[K80] Herc-1 NNNNN>, N=176.
Ref:	=1994ApJ...427L...9K
by	KOO D.C. , BERSHADY M.A., WIRTH G.D., STANFORD S.A., MAJEWSKI S.R.
	Astrophys. J., 427, 9-12 (1994)
	HST images of very compact blue galaxies at z about 0.2.
o	<[K80] Lynx-2 NNNNN> here N=3
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K80a]
[K80a]	(Kron, 1980)
*****	Avoid the usage of [K80a], prefer [K80]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K80b]
[K80b]	(Kurtanidze, 1980)
Write:	<<[K80b] NN>>
N:	21
Object:	Carbon * (SIMBAD class: C* = Carbon Star)
Stat:	is completely incorporated in Simbad
Ref:	=1980ATsir1109....2K
by	KURTANIDZE O.M.
	Astron. Tsirk., 1109, 2-6 (1980)
	New carbon stars in the selected Milky Way regions.
o	Identification charts
o	Table 2: <[K80b] NN> (Nos 1-21).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K82]
[K82]	(Keel, 1982)
Write:	<<[K82] Star NN>>
N:	15
Object:	* (SIMBAD class: Star)
Note:	Photoelectric sequence stars in the field of QSO 0957+561.
Ref:	=1982ApJ...255...20K
by	KEEL W.C.
	Astrophys. J., 255, 20-24 (1982)
	The nature of the light variations in the double QSO Q0957+561.
o	Fig.1, Table 1: <[K82] Star NN> (Nos 1-15).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K85]
[K85]	(Keel, 1985)
Write:	<<[K85] SGP N>>
N:	6 among 8
Object:	G (SIMBAD class: Galaxy)
Note:	N=8 suspected jet galaxies in the South Galactic Pole region
in source:	NAME SGP
Ref:	=1985AJ.....90.2207K
by	KEEL W.C.
	Astron. J., 90, 2207-2217 (1985)
	Recognition and classification of galaxies with optical jets.
o	Table II: <[K85] SGP N> N=6 among (Nos 1-8)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K88]
[K88]	(Kennicutt, 1988)= ([K88a])
Write:	<<[K88] NGC NNNN N>>
N:	32
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	N=32 HII regions in 11 NGC galaxies
Ref:	=1988ApJ...334..144K
by	KENNICUTT R.C.Jr
	Astrophys. J., 334, 144-158 (1988)
	Properties of H II region populations in galaxies. I. The first-ranked H II regions.
o	ST 1, 2 from 1974ApJ...191..603S and not from 1974ApJ...194..223S as given in the paper. In SIMBAD [ST74b] Ho I 1, 2
o	Table 4: <[K88] NGC NNNN N> N=32
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K88a]
[K88a]	(Kennicutt, 1988)
*****	Avoid the usage of [K88a], prefer [K88]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K88b]
[K88b]	(Kassim, 1988)
Write:	<<[K88b] LL.l+B.b>>
N:	79
Object:	Poss. SNR (SIMBAD class: SNRemnant_Candidate = SuperNova Remnant Candidate)
Stat:	is completely incorporated in Simbad
Ref:	=1988ApJ...328L..55K
by	KASSIM N.E.
	Astrophys. J., 328, 55-58 (1988)
	SNR candidates from the Clark Lake Galactic plane survey.
o	Table 1: <[K88b] LL.l+B.b> N=79
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: K90
K90	(Karachentsev+, 1990)
*****	Avoid the usage of K90, prefer [KK90]
Origin	of the Acronym: L = Found in the literature
Details on Acronym: [K92]
[K92]	(Kun, 1992)= (Kun)
Write:	<<[K92] NNN>>
N:	100
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Stat:	is completely incorporated in Simbad
Note:	Table 2. Identif. charts
Ref:	=1992A&AS...92..875K
by	KUN M.
	Astron. Astrophys., Suppl. Ser., 92, 875-884 (1992)
	A search for H-α emission stars in regions of highlatitude molecular clouds.
o	Table 2: <[K92] NNN> N=100
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K94]
[K94]	(Kim, 1994)= ([KKD94a])
Write:	<<[K94] HHMMSS.ss+DDMMSS.s>>
N:	299
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
in source:	Coma Cluster = ACO 1656
Ref:	=1994A&AS..105..385K
by	KIM K.-T. , KRONBERG P.P., DEWDNEY P.E., LANDECKER T.L.
	Astron. Astrophys., Suppl. Ser., 105, 385-401 (1994)
	Radio observations of the Coma cluster of galaxies and its immediate vicinity. I. Radio data and optical identifications.
o	Table 1: <10P NNN> (Nos 1-482). Table 8: <[K94] HHMMSS.ss+DDMMSS.s> N=107.
Ref:	=1994A&AS..105..403K
by	KIM K.-T.
	Astron. Astrophys., Suppl. Ser., 105, 403-413 (1994)
	Radio observations of the Coma cluster of galaxies and its immediate vicinity. II. A master list of radio sources.
o	Table 2: <[K94] HHMMSS.s+DDMMSS.s> N=298
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K95]
[K95]	(Klose, 1995)= ([K95a])
Write:	<<[K95] A>>
N:	4
Object:	Obj. (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Optical counterpart of 1B 911001.
Ref:	=1995ApJ...446..357K
by	KLOSE S.
	Astrophys. J., 446, 357-360 (1995)
	Search for an optical counterpart of the source of GRB 911001.
o	<[K95] A> (Nos A-D)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K95a]
[K95a]	(Klose, 1995)
*****	Avoid the usage of [K95a], prefer [K95]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K95b]
[K95b]	(Kohoutek, 1995)= (Kou)
Write:	<<[K95b] NN>>
N:	34
Object:	* (SIMBAD class: Star)
Note:	N=34 field stars (map Fig. 2) among (Nos 11-46)
Ref:	=1995A&AS..113..107K
by	KOHOUTEK L.
	Astron. Astrophys., Suppl. Ser., 113, 107-113 (1995)
	Study of the bipolar planetary nebula NGC 2346. I. Historical photometry of the central star.
o	Table 4: <[K95b] NN> N=34 among (Nos 11-44)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K96]
[K96]	(Kazlauskas, 1996)
Write:	<<[K96] NNN>>
N:	152
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
in source:	[K60] 217
Ref:	=1996BaltA...5..319K
by	KAZLAUSKAS A.
	Baltic Astronomy, 5, 319-335 (1996)
	Interstellar extinction in the dark cloud Khavtassi 217 in Cassiopeia.
o	[K96] 2 = HD 4625 = BD +65 97, not BD +66 97 as printed page 323.
o	Table 1: <[K96] NNN> (Nos 1-152)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K97]
[K97]	(Kishimoto, 1997) (Not yet in Simbad)
Write:	<<[K97] NN>>
N:	19
Object:	Clump (SIMBAD class: PartofG = Part of a Galaxy)
Note:	HST imaging polarimetry
in source:	NGC 1068
Ref:	=1997Ap&SS.248..277K
by	KISHIMOTO M.
	Astrophys. Space Sci., 248, 277-285 (1997)
	Clumpy structure and polarization in NGC 1068.
o	Table 1: <[K97] NN> (Nos 1-19)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K98]
[K98]	(Knude, 1998)= ([K98a])
Write:	<<[K98] JHHMMSS.ss+DDMMSS.ss>> <<[K98] JHHMMSS.ss+DDMMSS.s>>
N:	9
Object:	* (SIMBAD class: Star)
Stat:	is completely incorporated in Simbad
Note:	Tables 1, 2, 3: N=9 stars are without identifications, their coordinates are used as a format. See also [BBL98]
Ref:	=1998A&AS..130..477K
by	KNUDE J.
	Astron. Astrophys., Suppl. Ser., 130, 477-484 (1998)
	Stellar uvbyβ photometry in three EUV shadow directions.
o	Tables 1, 2, 3: <[K98] JHHMMSS.ss+DDMMSS.ss>, <[K98] JHHMMSS.ss+DDMMSS.s>, N=9
=E=	Catalogue in electronic form as J/A+AS/130/477
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K98a]
[K98a]	(Knude, 1998)
*****	Avoid the usage of [K98a], prefer [K98]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K98b]
[K98b]	(Kim, 1998)= (SG) (Not yet in Simbad)
Write:	<<[K98b] SG NN>>
Object:	Supergiant Shell (SIMBAD class: Unknown = Object of Unknown Nature)
Note:	From Kim S. Thesis, 1998, The Australian National University.
in source:	Magellanic Clouds:LMC = LMC
Ref:	=1999A&A...350..457E
by	EFREMOV Y.N. , EHLEROVA S., PALOUS J.
	Astron. Astrophys., 350, 457-468 (1999)
	Gamma ray bursts versus OB associations: do they trigger star formation?
o	N=2 'SG' from Kim Thesis, 1998.
o	<[K98b] SG NN> N=2 (Nos 8, 24).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K98c]
[K98c]	(Kun, 1998)
Write:	<<[K98c] Em* NNN>> <<[K98c] Core NNN>>
N:	142+107
Object:	Em* (SIMBAD class: EmLine* = Emission-line Star)
Note:	IRAS survey and Konkoly objective prism survey. N=142 H-alpha emission stars in the Cepheus region. N=107 CO cores in the Cepheus region.
in source:	NAME Cepheus Flare
Ref:	=1998ApJS..115...59K
by	KUN M.
	Astrophys. J., Suppl. Ser., 115, 59-89 (1998)
	Star formation in the Cepheus flare molecular clouds. I. Distance determination and the young stellar object candidates.
o	in ref list HERBIG 1988LicOB1111....1H instead of 1984
o	Table 3: <[K98c] Em* NNN> (Nos 1-142). Table 5: <[K98c] Core NNN> (Nos 1-107).
=E=	Catalogue in electronic form as J/ApJS/115/59
=E=	Catalogue in electronic form as <V/73A/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K98d]
[K98d]	(Knapen, 1998)
Write:	<<[K98d] NNNN>>
N:	1948
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	WHT TAURUS Hα observations of N=1948 HII regions in the disc of M100.
in source:	M 100 = NGC 4321
Ref:	=1998MNRAS.297..255K
by	KNAPEN J.H.
	Mon. Not. R. Astron. Soc., 297, 255-264 (1998)
	Statistical properties of H II regions in the disc of M100.
o	catalog: <[K98d] NNNN> (Nos 1-1948).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: K99
K99	(Kunkel, 1999)
*****	Avoid the usage of K99, prefer [KKL2000b]
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [K99]
[K99]	(Kahabka, 1999)= ([K99a]) = (SW)
Write:	<<[K99] SWa>> <<[K99] CNN>>
N:	42
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	ROSAT PSPC observations of M 31. In the format, the letters 'SW' stand for Supper and White, N=16 supersoft sources. In the format, the letter 'C' stands for Complementary, N=26 source from a complementary sample. (SWa-o from Supper et al ([SHP97],) (SWt from White et al (1995ApJ...445L.125W).) See also [SPH99]
in source:	M 31 = NGC 224
Ref:	=1999A&A...344..459K
by	KAHABKA P.
	Astron. Astrophys., 344, 459-471 (1999)
	The M 31 population of supersoft sources.
o	RX J0043.9+5148 misprint for RX J0043.9+4151.
o	Table 1: <[K99] SWa> (Nos SWa-SWo, SWt) N=16, <[K99] CNN> (Nos C17-C42).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K99a]
[K99a]	(Kahabka, 1999)
*****	Avoid the usage of [K99a], prefer [K99]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K99b]
[K99b]	(Knezek, 1999)= (HIPASS)
Write:	<<[K99b] HIPASS JHHMM+DD>>
N:	5
Object:	HI G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	See HIPASS.
in source:	NAME CEN A GROUP
Ref:	=1999PASA...16...60K
by	KNEZEK P.M.
	Publications - Astron. Soc. Australia, 16, 60-65 (1999)
	Optical counterparts to galaxies in the Cen A group discovered by HIPASS.
o	<[K99b] HIPASS JHHMM+DD> N=2.
Ref:	=1999ApJ...524..612B
by	BANKS G.D. , DISNEY M.J., KNEZEK P.M., JERJEN H., BARNES D.G., BHATAL R., DE BLOK W.J.G., BOYCE P.J., EKERS R.D., FREEMAN K.C., GIBSON B.K., HENNING P.A., KILBORN V., KORIBALSKI B., KRAAN-KORTEWEG R.C., MALIN D.F., MINCHIN R.F., MOULD J.R., OOSTERLOO T., PRICE R.M., PUTMAN M.E., RYDER S.D., SADLER E.M., STAVELEY-SMITH L., STEWART I., STOOTMAN F., VAILE R.A., WEBSTER R.L., WRIGHT A.E.
	Astrophys. J., 524, 612-622 (1999)
	New galaxies discovered in the first blind H I survey of the Centaurus A group.
o	Table 1: <[K99b] HIPASS JHHMM+DD> N=5, 3 are new.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [K99c]
[K99c]	(Kishimoto, 1999)
Write:	<<[K99c] NN>>
N:	30
Object:	Cloud (SIMBAD class: Cloud)
Stat:	is completely incorporated in Simbad
Note:	HST archival data. N=30 clouds in NGC 1068. Map in Fig.10.
in source:	NGC 1068.
Ref:	=1999ApJ...518..676K
by	KISHIMOTO M.
	Astrophys. J., 518, 676-692 (1999)
	The location of the nucleus of NGC 1068 and the three-dimensional structure of its nuclear region.
o	Table 3: <[K99c] NN> (Nos 1-30).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [K99d]
[K99d]	(Kaas, 1999)
Write:	<<[K99d] N-NN>> <<[K99d] YSO NN>>
N:	37+7+14+45+57
Object:	YSO (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Study of YSO in the Serpens Cloud Core region. Table 1: format '1-NN', sources with NIR excess. Tables 2-4: Sources that have varied photometrically during 2 period of measures. Table 5: new YSO. Map in Fig.2
in source:	NAME Serpens Cloud
Ref:	=1999AJ....118..558K
by	KAAS A.A.
	Astron. J., 118, 558-571 (1999)
	K-band variability as a method to select young stellar object candidates.
o	p. 562: FIRS = [HWJ84] FIRS 1.
o	Table 1: <[K99d] 1-NN> (Nos 1-1 to 1-37). Table 2: <[K99d] 2-N> (Nos 2-1 to 2-7). Table 3: <[K99d] 3-NN> (Nos 3-1 to 3-14). Table 4: <[K99d] 4-NN> (Nos 4-1 to 4-45). Table 5: <[K99d] YSO NN> (Nos 1-57).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Kö
Kö	(Königstuhl)
*****	Avoid the usage of Kö, prefer Koenigstuhl
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: Ka
Ka	(Kazarian)= Kaz = Kaza = (Kazarian)
Write:	<<Ka NNN>>
N:	702
Object:	G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Identif. charts
Ref:	=1979Afz....15....5K
by	KAZARIAN M.A.
	Astrofizika, 15, 5-18 (1979)
	New galaxies with ultraviolet excess. I.
o	Table 1: <Ka NNN> (Nos 1-136)
Ref:	=1979Afz....15..193K
by	KAZARIAN M.A.
	Astrofizika, 15, 193-200 (1979)
	New galaxies with ultraviolet excess. II.
o	Table 1: <Ka NNN> (Nos 137-241)
Ref:	=1980Afz....16...17K
by	KAZARIAN M.A. , KAZARIAN E.S.
	Astrofizika, 16, 17-23 (1980)
	New galaxies with ultraviolet excess. III.
o	Table 1: <Ka NNN> (Nos 242-352)
Ref:	=1982Afz....18..512K
by	KAZARIAN M.A. , KAZARIAN E.S.
	Astrofizika, 18, 512-522 (1982)
	New galaxies with ultraviolet excess. IV.
o	Ka 353-466
o	Table 2: <Ka NNN> (Nos 353-466)
Ref:	=1983Afz....19..213K
by	KAZARIAN M.A. , KAZARIAN E.S.
	Astrofizika, 19, 213-220 (1983)
	New galaxies with ultraviolet excess. V.
o	Table 1: <Ka NNN> (Nos 467-580)
Ref:	=2005Ap.....48..344K
by	KAZARIAN M.A. , PETROSIAN G.V.
	Astrophysics, 48, 344-354 (2005)
	New galaxies with UV excess. VI.
o	Table 1: <Ka NNN> (Nos 581-702).
=E=	Catalogue in electronic form as J/other/Ap/48.344
Origin	of the Acronym: L = Found in the literature
Details on Acronym: KA
KA	(Kiev Area)
*****	Avoid the usage of KA, prefer Kiev
Origin	of the Acronym: L = Found in the literature
Details on Acronym: KA
KA	(Ratnatunga K.A.)
*****	Avoid the usage of KA, prefer RKA
Origin	of the Acronym: L (1985AJ.....90.2244H)
Details on Acronym: Ka
Ka	(Kazarian)
*****	Avoid the usage of Ka, prefer Kj
Details on Acronym: [KA2008]
[KA2008]	(Kaaret+Alonso-Herrero, 2008)
Write:	<<[KA2008] NGC 4194 N>> <<[KA2008] NGC 7541 NN>> <<[KA2008] M 100 NN>> <<[KA2008] NGC 4945 NN>>
N:	6+15+50+48
Object:	(X) (SIMBAD class: X = X-ray Source)
Note:	Chandra observations of N=4 galaxies.
in source:	NGC 4194
in source:	NGC 7541
in source:	M 100 = NGC 4321
in source:	NGC 4945
Ref:	=2008ApJ...682.1020K
by	KAARET P. , ALONSO-HERRERO A.
	Astrophys. J., 682, 1020-1028 (2008)
	X-ray sources in the star-forming galaxies NGC 4194 and NGC 7541.
o	Table 2: <[KA2008] NGC 4194 N> (Nos 1-6). Table 3: <[KA2008] NGC 7541 NN> (Nos 1-15). Table 5: <[KA2008] M 100 NN> (Nos 1-50). Table 6: <[KA2008] NGC 4945 NN> (Nos 1-48).
=E=	Catalogue in electronic form as <J/ApJ/682/1020/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KA2010]
[KA2010]	(Kumar+Anandarao, 2010)
Write:	<<[KA2010] 0/I NN>> <<[KA2010] II NNN>>
N:	65+168
Object:	Poss. YSO (SIMBAD class: YSO_Candidate = Young Stellar Object Candidate)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC observations of N=65 class 0/I and 168 class II YSOs in the star-forming region M8.
in source:	M 8 = Lagoon Nebula
Ref:	=2010MNRAS.407.1170K
by	KUMAR D.L. , ANANDARAO B.G.
	Mon. Not. R. Astron. Soc., 407, 1170-1181 (2010)
	A study of the massive star-forming region M8 using images from the Spitzer Infrared Array Camera.
o	Table 1: <[KA2010] 0/I NN> (Nos 1-65). Table 2: <[KA2010] II NNN> (Nos 1-168).
=E=	Catalogue in electronic form as J/MNRAS/407/1170
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KA2020]
[KA2020]	(Kim+An, 2020)
Write:	<<[KA2020] R3>>
N:	1
Object:	(X) (SIMBAD class: X = X-ray Source)
Stat:	is completely incorporated in Simbad
Note:	N=1 X-ray source near PSR J1418-6058. Use of Chandra and XMM-Newton archival data. See also [NRR2005].
Ref:	=2020ApJ...892....5K
by	KIM M. , AN H.
	Astrophys. J., 892, 5-5 (2020)
	Characterizing X-ray properties of the γ-ray pulsar PSR J1418-6058 in the Rabbit pulsar wind nebula.
o	Fig. 1: <[KA2020] R3> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KAA2009]
[KAA2009]	(Kubo+Allam+Annis+, 2009)
Write:	<<[KAA2009] SDSS JHHMM+DDMM>> <<[KAA2009] SDSS JHHMM+DDMM lens>> <<[KAA2009] SDSS JHHMM+DDMM source>>
N:	6+6+6
Object:	Grav. lens system + Grav. lens + Lensed source (SIMBAD class: GravLensSystem = Gravitational Lens System (lens+images))
Stat:	is completely incorporated in Simbad
Note:	Apache Point Observatory 3.5m telescope spectroscopy and photometry of strongly lensed SDSS galaxies.
Ref:	=2009ApJ...696L..61K
by	KUBO J.M. , ALLAM S.S., ANNIS J., BUCKLEY-GEER E.J., DIEHL H.T., KUBIK D., LIN H., TUCKER D.
	Astrophys. J., 696L, 61-65 (2009)
	The Sloan bright arcs survey: six strongly lensed galaxies at z = 0.4-1.4.
o	Table 1: <[KAA2009] SDSS JHHMM+DDMM> N=6, <[KAA2009] SDSS JHHMM+DDMM source> N=6, <[KAA2009] SDSS JHHMM+DDMM lens> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KAA2020]
[KAA2020]	(Konyves+Andre+Arzoumanian+, 2020) (Not yet in Simbad)
Write:	<<[KAA2020] JHHMMSS.s+DDMMSS>>
N:	26
Object:	Poss. Dense Core (SIMBAD class: Infrared = Infra-Red Source)
Note:	N=26 candidate cores, possible extragalactic contaminants found in the study of Orion B, as part of the Herschel Gould Belt Survey (HGBS).
in source:	NAME Orion B
Ref:	=2020A&A...635A..34K
by	KONYVES V. , ANDRE P., ARZOUMANIAN D., SCHNEIDER N., MEN'SHCHIKOV A., BONTEMPS S., LADJELATE B., DIDELON P., PEZZUTO S., BENEDETTINI M., BRACCO A., DI FRANCESCO J., GOODWIN S., RYGL K.L.J., SHIMAJIRI Y., SPINOGLIO L., WARD-THOMPSON D., WHITE G.J.
	Astron. Astrophys., 635A, 34-34 (2020)
	Properties of the dense core population in Orion B as seen by the Herschel Gould Belt survey.
o	Tables A.1-A.2: <HGBS JHHMMSS.s+DDMMSS> N=1844. Table A.1: <[KAA2020] JHHMMSS.s+DDMMSS> N=26.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Kaas
Kaas	(Kaas+)
*****	Avoid the usage of Kaas, prefer [KOB2004]
Origin	of the Acronym: L (2007ApJ...669..493W)
Details on Acronym: [KAB2007]
[KAB2007]	(Kilic+Allende Prieto+Brown+, 2007)
Write:	<<[KAB2007] Cand NNN>>
N:	42 among 487
Object:	Poss. WD (SIMBAD class: WhiteDwarf_Candidate = White Dwarf Candidate)
Note:	MMT optical spectroscopy of white dwarf candidates.
Ref:	=2007ApJ...660.1451K
by	KILIC M. , ALLENDE PRIETO C., BROWN W.R., KOESTER D.
	Astrophys. J., 660, 1451-1461 (2007)
	The lowest mass white dwarf.
o	Table 1: <[KAB2007] Cand NNN> N=42 among (Nos 17-487).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KAC2002]
[KAC2002]	(Kanekar+Athreya+Chengalur, 2002)
Write:	<<[KAC2002] A>>
N:	1
Object:	G (SIMBAD class: EmissionG = Emission-line galaxy)
Stat:	is completely incorporated in Simbad
Note:	GMRT observations. Fig.2: Candidate 21cm absorber in the field of QSO 1243-072, identified with a galaxy.
Ref:	=2002A&A...382..838K
by	KANEKAR N. , ATHREYA R.M., CHENGALUR J.N.
	Astron. Astrophys., 382, 838-842 (2002)
	A new 21-cm absorber identified with an L~L^{} galaxy.*
o	Fig.2: <[KAC2002] A> (No. A).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KAC2006]
[KAC2006]	(Kassis+Adams+Campbell+, 2006)
Write:	<<[KAC2006] JHHMMSS.s+DDMMSS>>
N:	2+2
Object:	(Mid IR) (SIMBAD class: Infrared = Infra-Red Source)
Stat:	is completely incorporated in Simbad
Note:	Mid-IR observations using MIRSI in Orion nebula. Two new sources with no known counterpart and two new diffuse emission structures are found.
in source:	NAME Orion Nebula
Ref:	=2006ApJ...637..823K
by	KASSIS M. , ADAMS J.D., CAMPBELL M.F., DEUTSCH L.K., HORA J.L., JACKSON J.M., TOLLESTRUP E.V.
	Astrophys. J., 637, 823-837 (2006)
	Mid-infrared emission at photodissociation regions in the Orion nebula.
o	Paragr. 3.1.2: <[KAC2006] JHHMMSS.s+DDMMSS> N=4.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KAC93]
[KAC93]	(Knapen+Arnth-Jensen+Cepa+, 1993)
Write:	<<[KAC93] NNN>>
N:	735
Object:	HII (SIMBAD class: HIIReg = HII Region)
in source:	NGC 6814
Ref:	=1993AJ....106...56K
by	KNAPEN J.H. , ARNTH-JENSEN N., CEPA J., BECKMAN J.E.
	Astron. J., 106, 56-65 (1993)
	Statistics and properties of H II regions in NGC 6814.
o	Catalog: <[KAC93] NNN> (Nos 0-735, No. 716 missing).
=E=	Catalogue in electronic form as J/AJ/106/56
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: KACT
KACT	(Kepler ARPS Candidate Transit [ARPS= AutoRegressive Planet Search project]) >>>>>> New acronym being registered
Auth.:	Eric D. Feigelson
Origin	of the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym: [KAD2010]
[KAD2010]	(Kubo+Allam+Drabek+, 2010)
Write:	<<[KAD2010] SDSS JHHMM+DDMM>> <<[KAD2010] SDSS JHHMM+DDMM lens>> <<[KAD2010] SDSS JHHMM+DDMM source>>
N:	7+7+7+
Object:	Grav. lens system + Grav. lens + Grav. lensed image of a G (SIMBAD class: GravLensSystem = Gravitational Lens System (lens+images))
Stat:	is completely incorporated in Simbad
Note:	APO 3.5m telescope and KPNO Mayall 4m telescope spectroscopy of N=7 gravitational lens systems from the SDSS.
Ref:	=2010ApJ...724L.137K
by	KUBO J.M. , ALLAM S.S., DRABEK E., LIN H., TUCKER D., BUCKLEY-GEER E.J., DIEHL H.T., SOARES-SANTOS M., HAO J., WIESNER M., WEST A., KUBIK D., ANNIS J., FRIEMAN J.A.
	Astrophys. J., 724L, 137-142 (2010)
	The Sloan bright arcs survey: discovery of seven new strongly lensed galaxies from z = 0.66-2.94.
o	Table 1: <[KAD2010] SDSS JHHMM+DDMM> N=7, <[KAD2010] SDSS JHHMM+DDMM lens> N=7, <[KAD2010] SDSS JHHMM+DDMM source> N=7.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KAG2008]
[KAG2008]	(Koenig Allen+Gutermuth+, 2008)
Write:	<<[KAG2008] NNNNN>> <<[KAG2008] globule NN>> <<[KAG2008] gNNN>>
N:	17771+18+927
Object:	(IR)+star-forming globule+extragalactic sources (SIMBAD class: Infrared = Infra-Red Source)
Note:	Spitzer IRAC and MIPS observations of W 5.
in source:	W 5
Ref:	=2008ApJ...688.1142K
by	KOENIG X.P. , ALLEN L.E., GUTERMUTH R.A., HORA J.L., BRUNT C.M., MUZEROLLE J.
	Astrophys. J., 688, 1142-1158 (2008)
	Clustered and triggered star formation in W5: observations with Spitzer.
o	Parag. 4.3 : Object G138.295+1.555 = [DZC97] 25 in SIMBAD
o	Table 2: <[KAG2008] NNNNN> (Nos 1-17771). Table 4: <[KAG2008] globule NN> (Nos 1-18). Table 6: <[KAG2008] gNNN> (Nos g1-g927).
=E=	Catalogue in electronic form as <J/ApJ/688/1142/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KAG2014]
[KAG2014]	(Konstantopoulos+Appleton+Guillard+, 2014)
Write:	<<[KAG2014] NNNNN>>
N:	39
Object:	HII (SIMBAD class: HIIReg = HII Region)
Note:	Gemini GMOS spectroscopic observations of N=39 Hα-emitting regions in Stephan's Quintet (HCG 92). Use of archival HST WFC3 data.
in source:	NAME Stephan's Quintet
Ref:	=2014ApJ...784....1K
by	KONSTANTOPOULOS I.S. , APPLETON P.N., GUILLARD P., TRANCHO G., CLUVER M.E., BASTIAN N., CHARLTON J.C., FEDOTOV K., GALLAGHER S.C., SMITH L.J., STRUCK C.J.
	Astrophys. J., 784, 1 (2014)
	Shocks and star formation in Stephan's Quintet. I. Gemini spectroscopy of Hα-bright knots.
o	Table 1: <[KAG2014] NNNNN> N=39 among (Nos 10006-60011).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: KAIT
KAIT	(Katzman Automatic Imaging Telescope)
Write:	<<KAIT -YYA>> <<KAIT -YYaa>>
Object:	Transient (SIMBAD class: Transient = Transient Event)
Note:	Lick KAIT observations of transients. For more information, visit: http://w.astro.berkeley.edu/bait/kait.html
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [KAK2008]
[KAK2008]	(Koenig+Allen+Kenyon+, 2008)
Write:	<<[KAK2008] A>>
N:	4
Object:	Globule (SIMBAD class: ComGlob = Cometary Globule / Pillar)
Stat:	is completely incorporated in Simbad
Note:	Spitzer IRAC and MIPS observations of W5. N=3+1 dusty cometary globules near HD 17505 and HD 18326.
in source:	W 5
Ref:	=2008ApJ...687L..37K
by	KOENIG X.P. , ALLEN L.E., KENYON S.J., SU K.Y.L., BALOG Z.
	Astrophys. J., 687L, 37-40 (2008)
	Dusty cometary globules in W5.
o	Fig.2, Table 1: <[KAK2008] A> (Nos A-D).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KAM2010]
[KAM2010]	(Kravtsov+Alcaino+Marconi+, 2010)
Write:	<<[KAM2010] NNNN>>
N:	5481
Object:	* (SIMBAD class: Star)
Note:	Las Campanas Observatory Warsaw 1.3m telescope observations of the globular cluster NGC 1261.
in source:	NGC 1261
Ref:	=2010A&A...516A..23K
by	KRAVTSOV V. , ALCAINO G., MARCONI G., ALVARADO F.
	Astron. Astrophys., 516A, 23-23 (2010)
	Wide-field multi-color photometry of the galactic globular cluster NGC 1261.
o	photom.dat: <[KAM2010] NNNN> (Nos 1-5481).
=E=	Catalogue in electronic form as J/A+A/516/A23
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KAM2013]
[KAM2013]	(Koenig+Aalto+Muller+, 2013)
Write:	<<[KAM2013] GMA NN>>
N:	10
Object:	MCld (SIMBAD class: MolCld = Molecular Cloud)
Note:	Submillimeter Array (SMA) 12CO(2-1) and 13CO(2-1) observations of N=10 giant molecular associations in NGC 1614.
in source:	NGC 1614
Ref:	=2013A&A...553A..72K
by	KOENIG S. , AALTO S., MULLER S., BESWICK R.J., GALLAGHER III J.S.
	Astron. Astrophys., 553A, 72-72 (2013)
	The NGC 1614 interacting galaxy. Molecular gas feeding a ``ring of fire''.
o	Table 3: <[KAM2013] GMA NN> (Nos 1-10).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KAM2015]
[KAM2015]	(Koenyves+Andre+Men'shchikov+, 2015)
Write:	<<[KAM2015] NNN>>
N:	749
Object:	(FIR) (SIMBAD class: FarIR = Far-IR source (λ >= 30 µm))
Stat:	is completely incorporated in Simbad
Note:	N=749 starless dense cores and embedded protostars in the field of the Aquila molecular cloud complex. Use of PACS and SPIRE continuum data at 70µm to 500µm from the Herschel Gould Belt Survey. See also HGBS.
in source:	NAME Aql Rift
Ref:	=2015A&A...584A..91K
by	KOENYVES V. , ANDRE Ph., MEN'SHCHIKOV A., PALMEIRIM P., ARZOUMANIAN D., SCHNEIDER N., ROY A., DIDELON P., MAURY A., SHIMAJIRI Y., DI FRANCESCO J., BONTEMPS S., PERETTO N., BENEDETTINI M., BERNARD J.-P., ELIA D., GRIFFIN M.J., HILL T., KIRK J., LADJELATE B., MARSH K., MARTIN P.G., MOTTE F., NGUYEN LUONG Q., PEZZUTO S., ROUSSEL H., RYGL K.L.J., SADAVOY S.I., SCHISANO E., SPINOGLIO L., WARD-THOMPSON D., WHITE G.J.
	Astron. Astrophys., 584A, 91-91 (2015)
	A census of dense cores in the Aquila cloud complex: SPIRE/PACS observations from the Herschel Gould Belt survey.
o	Tables A.1-A.2, col(1): <[KAM2015] NNN> (Nos 1-749) = Tables A.1-A.2, col(2): <HGBS JHHMMSS.s+DDMMSS> N=749.
=E=	Catalogue in electronic form as J/A+A/584/A91
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KAM2019]
[KAM2019]	(Kong+Arce+Maureira+, 2019) (Not yet in Simbad)
Write:	<<[KAM2019] uN>>
N:	6
Object:	Dense Core (SIMBAD class: denseCore = Dense Core)
Note:	ALMA CO(2-1) observations of outflows associated with N=6 1.3 mm continuum cores in the infrared dark cloud G28.37+0.07.
in source:	NAME Dragon Nebula
Ref:	=2019ApJ...874..104K
by	KONG S. , ARCE H.G., MAUREIRA M.J., CASELLI P., TAN J.C., FONTANI F.
	Astrophys. J., 874, 104-104 (2019)
	Widespread molecular outflows in the infrared dark cloud G28.37+0.07: indications of orthogonal outflow-filament alignment.
o	Table 1: <[KAM2019] uN> (Nos u1 to u6).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KAM98]
[KAM98]	(Kneib+Alloin+Mellier+, 1998)
Write:	<<[KAM98] NN>>
N:	24
Object:	G (SIMBAD class: Galaxy)
Note:	Table 5: N=24 galaxies in the field of QSO 1413+1143. See also [KAP98].
Ref:	=1998A&A...329..827K
by	KNEIB J.-P. , ALLOIN D., MELLIER Y., GUILLOTEAU S., BARVAINIS R., ANTONUCCI R.
	Astron. Astrophys., 329, 827-839 (1998)
	Modelling the Cloverleaf: contribution of a galaxy cluster at z~1.7.
o	Table 5: <[KAM98] NN> (Nos 1-24)
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KAP98]
[KAP98]	(Kneib+Alloin+Pello, 1998)
Write:	<<[KAP98] HN>>
N:	2
Object:	G (SIMBAD class: Galaxy)
Note:	NICMOS-2 archival data. New elements in the identification of the Cloverleaf lens-system. No. H1 is the lensing galaxy. See also [KAM98].
in source:	NAME Cloverleaf
Ref:	=1998A&A...339L..65K
by	KNEIB J.-P. , ALLOIN D., PELLO R.
	Astron. Astrophys., 339, 65-68 (1998)
	Unveiling the nature of the Cloverleaf lens-system: HST/NICMOS-2 observations.
o	Table 2: <[KAP98] HN> (Nos H1-H2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: KaPa
KaPa	(Kazarian+Parsamian)
*****	Avoid the usage of KaPa, prefer KjPn
Details on Acronym: Kar
Kar	(Karachentseva)
*****	Avoid the usage of Kar, prefer K68
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Kar
Kar	(Karachentseva)
*****	Avoid the usage of Kar, prefer K73
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Kara
Kara	(Karachentseva)
*****	Avoid the usage of Kara, prefer K68
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Kara
Kara	(Karachentseva)
*****	Avoid the usage of Kara, prefer K73
Origin	of the Acronym: L (1997A&AS..124..109P)
Details on Acronym: Kara
Kara	(Karachentsev)
*****	Avoid the usage of Kara, prefer KPG
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Kara
Kara	(Karachentsev)
*****	Avoid the usage of Kara, prefer KPG
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Kara 68
Kara 68	(Karachentseva)
*****	Avoid the usage of Kara 68, prefer K68
Origin	of the Acronym: L (1997ApJS..111..233S)
Details on Acronym: Karachentsev
Karachentsev	(Karachentsev)
*****	Avoid the usage of Karachentsev, prefer KPG
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Karachentsev
Karachentsev	(Karachentsev)
*****	Avoid the usage of Karachentsev, prefer KPG
Origin	of the Acronym: L = Found in the literature
Details on Acronym: Karachentseva
Karachentseva	(Karachentseva)
*****	Avoid the usage of Karachentseva, prefer K68
Details on Acronym: Karmn
Karmn	(CARMENCITA)
Write:	<<Karmn JHHMMm+DDd>> <<Karmn JHHMMm+DDdW>> <<Karmn JHHMMm+DDdAAA>> <<Karmn JHHMMm+DDdWAAA>>
N:	∼2200
Object:	* (SIMBAD class: Star)
Note:	The CARMENCITA (CARMENES Cool dwarf Information and daTa Archive) input catalog contains approximately 2200 M dwarfs. CARMENES (Calar Alto high-Resolution search for M dwarfs with Exoearths with Near-infrared and optical Echelle Spectrographs) is a high-resolution spectrograph at the 3.5m Calar Alto telescope. Calar Alto 2.2m telescopes CAFOS and 1.5m Carlos Sanchez telescope FastCam spectroscopic observations, as part of the selection and characterisation of the sample of the CARMENES surveys. See website: http://carmenes.caha.es/
Ref:	=2015A&A...577A.128A
by	ALONSO-FLORIANO F.J. , MORALES J.C., CABALLERO J.A., MONTES D., KLUTSCH A., MUNDT R., CORTES-CONTRERAS M., RIBAS I., REINERS A., AMADO P.J., QUIRRENBACH A., JEFFERS S.V.
	Astron. Astrophys., 577A, 128-128 (2015)
	CARMENES input catalogue of M dwarfs. I. Low-resolution spectroscopy with CAFOS.
o	Tables A.1, A.2 A.3: <Karmn JHHMMm+DDd>, <Karmn JHHMMm+DDdW>, <Karmn JHHMMm+DDdWAAA> and <Karmn JHHMMm+DDdAAA> N=753.
Ref:	=2017A&A...597A..47C
by	CORTES-CONTRERAS M. , BEJAR V.J.S., CABALLERO J.A., GAUZA B., MONTES D., ALONSO-FLORIANO F.J., JEFFERS S.V., MORALES J.C., REINERS A., RIBAS I., SCHOFER P., QUIRRENBACH A., AMADO P.J., MUNDT R., SEIFERT W.
	Astron. Astrophys., 597A, 47-47 (2017)
	CARMENES input catalogue of M dwarfs. II. High-resolution imaging with FastCam.
o	Table A.1: <Karmn JHHMMm+DDdW> N=490.
=E=	Catalogue in electronic form as <J/A+A/577/A128/>
=E=	Catalogue in electronic form as <J/A+A/597/A47/>
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: KAT7HI
KAT7HI	(KAT-7 HI)
Write:	<<KAT7HI JHHMMSS+DDMMSS>>
N:	37
Object:	HI (SIMBAD class: HI = HI (21cm) Source)
Stat:	is completely incorporated in Simbad
Note:	N=37 detections in HI with KAT-7 in the Antlia Cluster, as part of spectral line commissioning of the Karoo Array Telescope (KAT-7).
in source:	NAME Antlia Cluster
Ref:	=2015MNRAS.452.1617H
by	HESS K.M. , JARRETT T.H., CARIGNAN C., PASSMOOR S.S., GOEDHART S.
	Mon. Not. R. Astron. Soc., 452, 1617-1636 (2015)
	KAT-7 science verification: cold gas, star formation, and substructure in the nearby Antlia Cluster.
o	Table 2: <KAT7HI JHHMMSS+DDMMSS> N=37.
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: [KAY2001]
[KAY2001]	(Kun+Aoyama+Yoshikawa+, 2001)
Write:	<<[KAY2001] N>> <<[KAY2001] GLLL.l+BB.b>>
N:	6
Object:	Cloud (SIMBAD class: MolCld = Molecular Cloud)
Stat:	is completely incorporated in Simbad
Note:	N=6 CO clouds in the region of IC 2118.
Ref:	=2001PASJ...53.1063K
by	KUN M. , AOYAMA H., YOSHIKAWA N., KAWAMURA A., YONEKURA Y., ONISHI T., FUKUI Y.
	Publ. Astron. Soc. Jap., 53, 1063-1070 (2001)
	Study of molecular clouds and star formation in the region of IC 2118.
o	Table 1: <[KAY2001] N> (Nos 1-6) = <[KAY2001] GLLL.l+BB.b> N=6.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: Kaz
Kaz	(Kazarian)
====>	Equivalent to: Ka
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: Kaza
Kaza	(Kazarian)
====>	Equivalent to: Ka
Origin	of the Acronym: L (1997A&AS..124..109P)
Details on Acronym: Kazarian
Kazarian	(Kazarian)
*****	Avoid the usage of Kazarian, prefer Ka
Origin	of the Acronym: D = Assigned by the Dictionary of Acronyms
Details on Acronym: KAZF
KAZF	(Kissler-Patig+Ashman+Zepf+Freeman)
Write:	<<KAZF 4565-NN>> <<KAZF 5907-NN>>
N:	40+25
Object:	GlCl (SIMBAD class: GlobCluster = Globular Cluster)
Stat:	is completely incorporated in Simbad
Note:	HST observations. Study of globular systems of the 2 galaxies NGC 4565 and NGC 5907.
in source:	NGC 4565
in source:	NGC 5907
Ref:	=1999AJ....118..197K
by	KISSLER-PATIG M. , ASHMAN K.M., ZEPF S.E., FREEMAN K.C.
	Astron. J., 118, 197-207 (1999)
	Hubble Space Telescope imaging of globular clusters in the edge-on spiral galaxies NGC 4565 and NGC 5907.
o	Table 2: <KAZF 4565-NN> (Nos 1-40). Table 3: <KAZF 5907-NN> (Nos 1-25).
Origin	of the Acronym: A = Assigned by the author(s)
Details on Acronym: KB
KB	(Kamper+van den Bergh)= (FBG) = (FMF) = (QSF)
Write:	<<KB Star NN>> <<KB QSF ANNw>> <<KB MK NNN>> <<KB F1a>>
N:	12+47+121+12
Object:	Knot (SIMBAD class: PartofCloud = Part of Cloud)
Note:	Reference stars, format 'star NN'. Quasi Stellar Flocculi, format 'QSF ANNw', some with several directions (n, s, w, e, or c). Supersedes [V71b] QSF ANN. Moving Knots, format MK NNN. Supersedes [V70] NN. See also FMF. Knots in filament 1 (=[BM54] Cas 1), format F1a.
in source:	NAME Cas A
Ref:	=1976ApJS...32..351K
by	KAMPER K. , VAN DEN BERGH S.
	Astrophys. J., Suppl. Ser., 32, 351-366 (1976)
	Optical studies of Cassiopeia A. V. A definitive study of proper motions.
o	Filament 1 = [BM54] Cas 1
o	Table 2: <KB Star NN> (Nos 1-12). Table 3: <KB QSF ANNw> (Nos R01-R30), N=35 (supersedes '[V71b] QSF ANN'). Table 4: <KB MK NNN> (Nos 1-117) (supersedes '[V70] NN'). Table 8: <KB F1a> N=12 among (Nos F1a and F1p)
Ref:	=1985ApJ...293..537V
by	VAN DEN BERGH S. , KAMPER K.
	Astrophys. J., 293, 537-541 (1985)
	Optical studies of Cassiopeia A. VII. Recent observations of the structure and evolution of the nebulosity.
o	Table 2: <KB QSF ANNw> (Nos R31-R40) 12 are new
Ref:	=1988ApJ...329L..89F
by	FESEN R.A. , BECKER R.H., GOODRICH R.W.
	Astrophys. J., 329, 89-92 (1988)
	Highest velocity ejecta of Cassiopeia A.
o	Table 1: <FMF NN> (Nos 10-15) added. p.L91: <KB MK NNN> (Nos 118-121) added.
Ref:	=2001AJ....122.2644F
by	FESEN R.A. , MORSE J.A., CHEVALIER R.A., BORKOWSKI K.J., GERARDY C.L., LAWRENCE S.S., VAN DEN BERGH S.
	Astron. J., 122, 2644-2661 (2001)
	Hubble space telescope WFPC2 imaging of Cassiopeia A.
o	<KB QSF RNN> (No. R41) added.
Origin	of the Acronym: L (1979ApJ...233..154C)
Details on Acronym: [KB2007]
[KB2007]	(Kelly+Bechtold, 2007)
Write:	<<[KB2007] JHHMMSS.s+DDMMSS.s>>
N:	100
Object:	Poss. Black Hole (SIMBAD class: BlackHole_Candidate = Black Hole Candidate)
Stat:	is completely incorporated in Simbad
Note:	Black hole mass estimates based on archival UV/optical spectra and new optical spectra observed at the 2.3m Bok telescope at Kitt Peak.
Ref:	=2007ApJS..168....1K
by	KELLY B.C. , BECHTOLD J.
	Astrophys. J., Suppl. Ser., 168, 1-18 (2007)
	Virial masses of black holes from single epoch spectra of active galactic nuclei.
o	Table 5: <[KB2007] JHHMMSS.s+DDMMSS.s> N=100.
=E=	Catalogue in electronic form as J/ApJS/168/1
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KB61]
[KB61]	(Kharadze+Bartaya, 1961)
Write:	<<[KB61] +DD NNN>>
N:	359+1268+775
Object:	* (SIMBAD class: Star)
Note:	N=359+1268+775 stars in the fields of N=3 open clusters NGC 6604, NGC 6913 and Trumpler 1.
in source:	NGC 6604
in source:	NGC 6913
in source:	Cl Trumpler 1
Ref:	=1961AbaOB..26...35K
by	KHARADZE E.K. , BARTAYA R.A.
	AbaOB, 26, 35 (1961)
	Spectra of stars near NGC 6604, NGC 6913, and Trumpler 1.
o	Table 2: <[KB61] +DD NNN> N=359+1268+775.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KB94]
[KB94]	(Kuchar+Bania, 1994)
Write:	<<[KB94] NN>>
N:	76
Object:	HII (SIMBAD class: HIIReg = HII Region)
Stat:	is completely incorporated in Simbad
Note:	Table 1: 19 sources among the 76 are from paper I: 1990ApJ...352..192K
Ref:	=1994ApJ...436..117K
by	KUCHAR T.A. , BANIA T.M.
	Astrophys. J., 436, 117-124 (1994)
	Kinematic distances of galactic HII regions from H I absorption studies.
o	<[KB94] NN> N=76
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KB98]
[KB98]	(Knezek+Bregman, 1998)= ([KB98a])
Write:	<<[KB98] QSO JHHMM+DDd>> <<[KB98] Obj JHHMMSS+DDMMSS>>
N:	21+46
Object:	? (SIMBAD class: Unknown = Object of Unknown Nature)
Stat:	is completely incorporated in Simbad
Note:	Use of ROSAT archive images of galaxies and clusters to search for QSO. Table 1: N=21 QSO, format 'QSO JHHMM+DDd'. Table 2: N=46 non-emission-line Objects, format 'Obj JHHMMSS+DDMMSS'. Finding charts for the QSO
Ref:	=1998AJ....115.1737K
by	KNEZEK P.M. , BREGMAN J.N.
	Astron. J., 115, 1737-1744 (1998)
	The identification of quasars behind elliptical galaxies and clusters of galaxies.
o	Table 1: QSO 0107-156 and QSO 1124+271 have a format with 1950 coordinates. Others QSO are '[KB98]', they have a format with 2000 coordinates.
o	Table 1: <[KB98] QSO JHHMM+DDd> N=20. Table 2: <[KB98] Obj JHHMMSS+DDMMSS> N=46.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KB98a]
[KB98a]	(Knezek+Bregman, 1998)
*****	Avoid the usage of [KB98a], prefer [KB98]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KB98b]
[KB98b]	(Koekemoer+Bicknell, 1998) (Not yet in Simbad)
Write:	<<[KB98b] Central>> <<[KB98b] Tail>> <<[KB98b] Cloud AN>>
N:	1+1+5
Object:	Part of G (SIMBAD class: PartofG = Part of a Galaxy)
Note:	Observations of the radio galaxy PKS 2356-61: N=2 components, 'Central' and 'Tail'. The Tail itself consists of 3 distinct clouds (Nos A-C), cloud B being composed of 2 components (Nos B1-B2).
in source:	PKS 2356-61
Ref:	=1998ApJ...497..662K
by	KOEKEMOER A.M. , BICKNELL G.V.
	Astrophys. J., 497, 662-680 (1998)
	Dynamics and excitation of radio galaxy emission-line regions. I. PKS 2356-61.
o	<[KB98b] Central> N=1, <[KB98b] Tail> N=1, <[KB98b] Cloud AN> (Nos A-C, B1-B2).
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KBA2019]
[KBA2019]	(Kos+Bland-Hawthorn+Asplund+, 2019)
Write:	<<[KBA2019] ASCC 21a>>
N:	1
Object:	Cluster of * (SIMBAD class: Cluster* = Cluster of Stars)
Stat:	is completely incorporated in Simbad
Note:	N=1 stellar overdensity in Gaia DR2 data in the Orion Complex. Use of GALAH DR2 and APOGEE DR14 data.
in source:	NAME Ori Complex
Ref:	=2019A&A...631A.166K
by	KOS J. , BLAND-HAWTHORN J., ASPLUND M., BUDER S., LEWIS G.F., LIN J., MARTELL S.L., NESS M.K., SHARMA S., DE SILVA G.M., SIMPSON J.D., ZUCKER D.B., ZWITTER T., COTAR K., SPINA L.
	Astron. Astrophys., 631A, 166-166 (2019)
	Discovery of a 21 Myr old stellar population in the Orion complex.
o	Fig. 2, Table 1: <[KBA2019] ASCC 21a> N=1.
=E=	Catalogue in electronic form as J/A+A/631/A166
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KBB2008]
[KBB2008]	(Kauffmann+Bertoldi+Bourke+, 2008)
Write:	<<[KBB2008] LNNNN CN>> <<[KBB2008] LNNNNA CN>> <<[KBB2008] LNNNNA-N CN>> <<[KBB2008] LNNNN-N CN>> <<[KBB2008] B18-N CN>> <<[KBB2008] TMC-N CN>> <<[KBB2008] TMC-NA CN>> <<[KBB2008] IRAS05413 CN>> <<[KBB2008] CB188 CN>> <<[KBB2008] Bern48 CN>> <<[KBB2008] LNNNN PN>> <<[KBB2008] LNNNNA PN>> <<[KBB2008] LNNNNA-N PN>> <<[KBB2008] LNNNN-N PN>> <<[KBB2008] B18-N PN>> <<[KBB2008] TMC-N PN>> <<[KBB2008] TMC-NA PN>> <<[KBB2008] IRAS05413 PN>> <<[KBB2008] CB188 PN>> <<[KBB2008] Bern48 PN>>
N:	86+108
Object:	Subcore + Em. Peak (SIMBAD class: PartofCloud = Part of Cloud)
Note:	MAMBO bolometer observations of small molecular clouds and cores.
Ref:	=2008A&A...487..993K
by	KAUFFMANN J. , BERTOLDI F., BOURKE T.L., EVANS II N.J., LEE C.W.
	Astron. Astrophys., 487, 993-1017 (2008)
	MAMBO mapping of Spitzer c2d small clouds and cores.
o	Table 3: <[KBB2008] LNNNN CN>, <[KBB2008] LNNNNA CN>, <[KBB2008] LNNNNA-N CN>, <[KBB2008] LNNNN-N CN>, <[KBB2008] B18-N CN>, <[KBB2008] TMC-N CN>, <[KBB2008] TMC-NA CN>, <[KBB2008] IRAS05413 CN>, <[KBB2008] CB188 CN>, <[KBB2008] Bern48 CN>, <[KBB2008] LNNNN PN>, <[KBB2008] LNNNNA PN>, <[KBB2008] LNNNNA-N PN>, <[KBB2008] LNNNN-N PN>, <[KBB2008] B18-N PN>, <[KBB2008] TMC-N PN>, <[KBB2008] TMC-NA PN>, <[KBB2008] IRAS05413 PN>, <[KBB2008] CB188 PN>, <[KBB2008] Bern48 PN> N=86+108..
=E=	Catalogue in electronic form as <J/A+A/487/993/>
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KBB2014]
[KBB2014]	(Kirby+Bullock+Boylan-Kolchin+, 2014)
Write:	<<[KBB2014] Cetus M05-NNNN>>
N:	120
Object:	RGB* (SIMBAD class: RGB* = Red Giant Branch star)
Note:	Keck DEIMOS spectroscopy of red giant stars in nearby dwarf galaxies. See also [KGS2010], [KCB2012], [BCG2013].
in source:	NAME Cetus Dwarf Galaxy
Ref:	=2014MNRAS.439.1015K
by	KIRBY E.N. , BULLOCK J.S., BOYLAN-KOLCHIN M., KAPLINGHAT M., COHEN J.G.
	Mon. Not. R. Astron. Soc., 439, 1015-1027 (2014)
	The dynamics of isolated Local Group galaxies.
o	Table 2: <[KBB2014] Cetus M05-NNNN> N=120 among (Nos 3371-3602). Table 2: <[KCG2013] IC 1613 B07-NNNNN> N=19 added, <[KCG2013] NGC 6822 M07-NNNNN> N=36 added, <[KCG2013] Peg NNNNNN> N=10 added, <[KCG2013] LeoA NNNNN> N=10 among (Nos 29587-34130) added, <[KCG2013] Aqr NNNN> N=18 added, <[KCB2012] NNNNN> N=33 added.
=E=	Catalogue in electronic form as J/MNRAS/439/1015
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KBB2019]
[KBB2019]	(Knowles+Baker+Bond+, 2019)= ([KBB2019a])
Write:	<<[KBB2019] ACT-CL JHHMM.m+DDMM A>> <<[KBB2019] ACT-CL JHHMM.m+DDMM WW>> <<[KBB2019] ACT-CL J0256.5+0006 RH>> <<[KBB2019] ACT-CL J0014.9-0057 CE>>
N:	50+3+1+1
Object:	(Rad) (SIMBAD class: Radio = Radio Source)
Stat:	is completely incorporated in Simbad
Note:	GMRT 610 MHz observations of N=50+3+1+1 radio sources in 10 Atacama Cosmology Telescope (ACT) clusters. In the formats, CE stands for "central emission", and RH possibly for "radio halo".
Ref:	=2019MNRAS.486.1332K
by	KNOWLES K. , BAKER A.J., BOND J.R., GALLARDO P.A., GUPTA N., HILTON M., HUGHES J.P., INTEMA H., LOPEZ-CARABALLO C.H., MOODLEY K., SCHMITT B.L., SIEVERS J., SIFON C., WOLLACK E.
	Mon. Not. R. Astron. Soc., 486, 1332-1349 (2019)
	GMRT 610 MHz observations of galaxy clusters in the ACT equatorial sample.
o	Figs 1, 3-11, Tables 3, 5-13: <[KBB2019] ACT-CL JHHMM.m+DDMM A> N=50, <[KBB2019] ACT-CL JHHMM.m+DDMM WW> N=3, <[KBB2019] ACT-CL J0256.5+0006 RH> N=1, <[KBB2019] ACT-CL J0014.9-0057 CE> N=1.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KBB2019a]
[KBB2019a]	(Knowles+Baker+Bond+, 2019) (Not yet in Simbad)
*****	Avoid the usage of [KBB2019a], prefer [KBB2019]
Origin	of the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: [KBB2019b]
[KBB2019b]	(Khullar+Bleem+Bayliss+, 2019)
Write:	<<[KBB2019b] JHHMMSS.sss+DDMMSS.ss>> <<[KBB2019b] JHHMMSS.sss+DDMMSS.sss>>
N:	44+22+3
Object:	G in ClG + G (SIMBAD class: Galaxy)
Stat:	is completely incorporated in Simbad
Note:	Magellan Clay 6.5-m telescope LDSS3C spectroscopy of N=44+25 galaxies, in the fields of 5 galaxy clusters (SPT-CL J2341-5724, SPT-CL J0156-5541, SPT-CL J0640-5113, SPT-CL J0607-4448, SPT-CL J0313-5334). In format "JHHMMSS.sss+DDMMSS.sss", the suffix "s" stands for "serendipitous", as in three instances, another galaxy fell serendipitously onto the slit.
in source:	SPT-CL J2341-5724
in source:	SPT-CL J0156-5541
in source:	SPT-CL J0640-5113
in source:	SPT-CL J0607-4448
in source:	SPT-CL J0313-5334
Ref:	=2019ApJ...870....7K
by	KHULLAR G. , BLEEM L.E., BAYLISS M.B., GLADDERS M.D., BENSON B.A., McDONALD M., ALLEN S.W., APPLEGATE D.E., ASHBY M.L.N., BOCQUET S., BRODWIN M., BULBUL E., CANNING R.E.A., CAPASSO R., CHIU I., CRAWFORD T.M., DE HAAN T., DIETRICH J.P., GONZALEZ A.H., HLAVACEK-LARRONDO J., HOEKSTRA H., HOLZAPFEL W.L., VON DER LINDEN A., MANTZ A.B., PATIL S., REICHARDT C.L., SARO A., SHARON K., STALDER B., STANFORD S.A., STARK A.A., STRAZZULLO V.
	Astrophys. J., 870, 7-7 (2019)
	Spectroscopic confirmation of five galaxy clusters at z > 1.25 in the 2500 °^{2} SPT-SZ survey.
o	Tables 3-4: <[KBB2019b] JHHMMSS.sss+DDMMSS.ss> N=44+22, <[KBB2019b] JHHMMSS.sss+DDMMSS.sss> N=3.
Origin	of the Acronym: S = Created by Simbad, the CDS Database
1 *Stopped after 9999 entries**

Dictionary of Nomenclature of Celestial Objects(Last update: 26-Apr-2024)

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Dictionary of Nomenclature of Celestial Objects
(Last update: 26-Apr-2024)

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