Dictionary of Nomenclature of Celestial Objects
(Last update: 22-Oct-2021)

Result of query: info cati Mrk$
 N> (Nos    1-20)
 Auth.:MILLER B.W.

Details on Acronym:   [M97a]
   [M97a] (Mighell, 1997) (Not yet in Simbad) Write:<<[M97a] Nyyyyxxxx>> N: 3302 Object:*  (SIMBAD class: Star) Note:HST WFPC2 observations.
Table 2: stellar photometry in the central region of the Carina Dwarf Galaxy.
In the format 'Nyyyyxxxx', 'N' stands for the WFPC2 chip (2, 3, or 4), the right-mos plete catalog will be available in summer 2001 (technical contact: Juan Cabanela, ) In the final archived MAPS, all O and E objects are cross-identified.
The fields are identified by their 3 digit POSS-I field designation, and the object ID number is the O emulsion "starnum", a number generated during the scanning process and guaranteed to be unique for each object in a fie for objects in previous catalogs (MAPS-NGP and MAPS-PP) were in a different format.
However, since each E and O emulsion number corresponds to a single POSS-I field, it will be a simple matter to map out each of those objects to its "new" MAPS designation. The "starnum" in those cases (used in the NNNNNNN portion of both the "old" and "new" designations) will be identical.
It is recommended that any future catalogs using a subset of the MAPS archive data, either use the existing MAPS designations or if new acronyms are used, the designations should follow a similar format, namely MAPS-AA PFFF-NNNNNNN or MAPS-AAA PFFF-NNNNNNN or MAPS-AAAA PFFF-NNNNNNN where the POSS-I field number and O-emulsion "starnum" ID are used. The AA, AAA, or AAAA refers to the nature of the subfield, type of object, or to the initials of the authors' last names (and is unique - i.e. it does not already appear in the Dictionary of Nomenclature of Celestial Objects). It is recommended that any such new acronyms be pre-registered with the IAU, using the form at http://cdsweb.u-strasbg.fr/viz-bin/DicForm. Ref:=2004AJ....127.1567P byPARKER J.E. , HUMPHREYS R.M., BEERS T.C. Astron. J., 127, 1567-1578 (2004) The asymmetric thick disk: a star-count and kinematic analysis. II. The kinematics. oTable 4: <MAPS AFFF-NNNNNNN> N=741. =E=Catalogue in electronic form as J/AJ/127/1567 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   MAPS-CD
   MAPS-CD (Minnesota Automated Plate Scanner, Cabanela+Dickey) Write:<<MAPS-CD PFFF-NNNNNNN>> N: 71 Object:HI G  (SIMBAD class: Galaxy) Stat:is completely incorporated in Simbad Note:Catalog of HI-rich galaxies selected from the MAPS catalog. The name 'MAPS-CD' is constructed following MAPS authors recommandations. Ref:=2002AJ....124...78C byCABANELA J.E. , DICKEY J.M. Astron. J., 124, 78-99 (2002) Galaxies on the blue edge. oTable 2: <MAPS-CD AFFF-NNNNNNN> N=71. Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   MAPS-NGP
   MAPS-NGP (Minnesota Automated Plate Scanner, NGP)= (MAP-NGP) Write:<<MAPS-NGP O-FFFF-NNNNNNNA>>
<<MAPS-NGP E-FFFF-NNNNNNNA>>
<<MAPS-NGP JHHMMSS.s+DDMMSS>> Object:G  (SIMBAD class: Galaxy) Note:The MAPS-NGP (Minnesota Automated Plate Scanner North Galactic Pole) Catalog is a diameter-limited catalog of all galaxies greater than 10 arcseconds in diameter on Palomar Sky Survey (Epoch I) plates within 30 degrees of the North Galactic Pole.
More information available here: http://astronomy.mnstate.edu/cabanela/research/MAPSNGP/
In the format, 'O' and 'E' stand for the plate image, 'FFFF' for plate number.
See MAPS. in source:NAME NGP Ref:=2001ApJ...550L..35B byBARTON E.J. , VAN ZEE L. Astrophys. J., 550, 35-38 (2001) Possible local spiral galaxy counterparts to compact blue galaxies at intermediate redshift. o1st ref. with <MAPS-NGP O-FFFF-NNNNNNNA> N=1. =E=Catalogue in electronic form as VII/214 Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   MAPS-PP
   MAPS-PP (Minnesota Automated Plate Scanner, Pisces Perseus) Write:<<MAPS-PP O-FFFF-NNNNNNNA>>
<<MAPS-PP E-FFFF-NNNNNNNA>> N: 1400 Object:G  (SIMBAD class: Galaxy) Stat:is completely incorporated in Simbad Note:From the MAPS survey. G in the Pisces-Perseus Supercluster. In the format, the letter 'A' stands for 'O' and 'E' plate, 'A-FFFF' for plate number. See MAPS. in source:NAME PPS Ref:=1998AJ....116.1094C byCABANELA J.E. , ALDERING G. Astron. J., 116, 1094-1117 (1998) Galaxy alignments in the Pisces-Perseus supercluster revisited. oTable 2: <MAPS-PP A-FFFF-NNNNNNNA> N=1400. =E=Catalogue in electronic form as J/AJ/116/1094 Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   MARD
   MARD (Multi-component mAtch filter RASS cluster confirmed using DES data) I added) Write:<<MARD JHHMMSS.s+DDMMSS>> N: 2950  (SIMBAD class: ClG = Cluster of Galaxies) Note:This acronym is meant to name clusters of the MARD-Y3 catalog of galaxy clusters described in Klein+19.
Cluster candidates were drawn from the RASS based 2RXS catalog (Boller+16) and identified using the MCMF method and DES-Y3 optical data. The naming convention follows that used in Boller et al. (2016A&A...588A.103B), replacing 2RXS with MARD for confirmed clusters. Ref:=2019MNRAS.488..739K byKLEIN M. , GRANDIS S., MOHR J.J., PAULUS M., ABBOTT T.M.C., ANNIS J., AVILA S., BERTIN E., BROOKS D., BUCKLEY-GEER E., CARNERO ROSELL A., CARRASCO KIND M., CARRETERO J., CASTANDER F.J., CUNHA C.E., D'ANDREA C.B., DA COSTA L.N., DE VICENTE J., DESAI S., DIEHL H.T., DIETRICH J.P., DOEL P., EVRARD A.E., FLAUGHER B., FOSALBA P., FRIEMAN J., GARCIA-BELLIDO J., GAZTANAGA E., GILES P.A., GRUEN D., GRUENDL R.A., GSCHWEND J., GUTIERREZ G., HARTLEY W.G., HOLLOWOOD D.L., HONSCHEID K., HOYLE B., JAMES D.J., JELTEMA T., KUEHN K., KUROPATKIN N., LIMA M., MAIA M.A.G., MARCH M., MARSHALL J.L., MENANTEAU F., MIQUEL R., OGANDO R.L.C., PLAZAS A.A., ROMER A.K., ROODMAN A., SANCHEZ E., SCARPINE V., SCHINDLER R., SERRANO S., SEVILLA-NOARBE I., SMITH M., SMITH R.C., SOARES-SANTOS M., SOBREIRA F., SUCHYTA E., SWANSON M.E.C., TARLE G., THOMAS D., VIKRAM V., (The DES Collaboration) Mon. Not. R. Astron. Soc., 488, 739-769 (2019) A new RASS galaxy cluster catalogue with low contamination extending to z ~ 1 in the DES overlap region. o<MARD JHHMMSS.s+DDMMSS> N=2950.

LMU Munich, Germany =E=Catalogue in electronic form as <J/MNRAS/488/739/> Originof the Acronym: p = Pre-registered to IAU Comm.5
Details on Acronym:   Mark
   Mark (Markarian) ***** Avoid the usage of Mark, prefer Mrk
Details on Acronym:   Mark
   Mark (Markarian) ***** Avoid the usage of Mark, prefer [L92b] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   Mark
   Mark (Markarian) ====>Equivalent to: Mrk
Details on Acronym:   Markarian
   Markarian (Markarian) ***** Avoid the usage of Markarian, prefer Mrk
Details on Acronym:   Markarian
   Markarian (Markarian)
Details on Acronym:   [MJR2015]
   [MJR2015] (Montillaud+Juvela+Rivera-Ingraham+, 2015) Write:<<[MJR2015] NNNN>> N: 4466 Object:(IR)  (SIMBAD class: IR = Infra-Red source) Stat:is completely incorporated in Simbad Note:Catalogue of N=4466 submillimeter sources within the clouds in 116 fields observed with the Herschel PACS and SPIRE instruments. Ref:=2015A&A...584A..92M byMONTILLAUD J. , JUVELA M., RIVERA-INGRAHAM A., MALINEN J., PELKONEN V.-M., RISTORCELLI I., MONTIER L., MARSHALL D.J., MARTON G., PAGANI L., TOTH L.V., ZAHORECZ S., YSARD N., McGEHEE P., PALADINI R., FALGARONE E., BERNARD J.-P., MOTTE F., ZAVAGNO A., DOI Y. Astron. Astrophys., 584A, 92-92 (2015) Galactic cold cores. IV. Cold submillimetre sources: catalogue and statistical analysis. oTable B.1 (gccscat.dat): <[MJR2015] NNNN> (Nos 1-4466). =E=Catalogue in electronic form as J/A+A/584/A92 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [MJS2008]
   [MJS2008] (Merin+Jorgensen+Spezzi+, 2008) Write:<<[MJS2008] NNN>> N: 159 Object:Poss. YSO  (SIMBAD class: YSO = Young Stellar Object) Stat:is completely incorporated in Simbad Note:Spitzer IRAC c2d observations to search for YSO candidates in Lupus I, III, et IV clouds. in source:NAME Lupus I = Lupus 1 in source:NAME Lupus III = Lupus 3 in source:NAME Lupus IV = Lupus 4 Ref:=2008ApJS..177..551M byMERIN B. , JORGENSEN J., SPEZZI L., ALCALA J.M., EVANS II N.J., HARVEY P.M., PRUSTI T., CHAPMAN N., HUARD T., VAN DISHOECK E.F., COMERON F. Astrophys. J., Suppl. Ser., 177, 551-583 (2008) The Spitzer c2d survey of large, nearby, interstellar clouds. XI. Lupus observed with IRAC and MIPS. oParagr. 5.2: IRAS 15589-4134 is a misprint for IRAS 15589-4132 oTable 5: <[MJS2008] NNN> (Nos 1-159). =E=Catalogue in electronic form as J/ApJS/177/551 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [MJS2009]
   [MJS2009] (Mao+Johnston-Hollitt+Stevens+, 2009) Write:<<[MJS2009] A>>
<<[MJS2009] JHHMMSS+DDMMSS>> N: 5+5 Object:Radio G  (SIMBAD class: RadioG = Radio Galaxy) Stat:is completely incorporated in Simbad Note:ATCA 1.4GHz observations of head-tail galaxies in the central region of the Horologium-Reticulum Supercluster. Ref:=2009MNRAS.392.1070M byMAO M.Y. , JOHNSTON-HOLLITT M., STEVENS J.B., WOTHERSPOON S.J. Mon. Not. R. Astron. Soc., 392, 1070-1079 (2009) Head-tail galaxies: beacons of high-density regions in clusters. oFig. 3, Table 2: <[MJS2009] A> (Nos A-E). Table 8: <[MJS2009] JHHMMSS+DDMMSS> N=5. Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   MJV
   MJV (mJIVE-20) Write:<<MJV NNNNN>> N: 21396 Object:(Rad)  (SIMBAD class: Radio = Radio-source) Note:Catalog of N=21396 compact radio sources as part of the mJy Imaging VLBA Exploration at 20cm (mJIVE-20).

The mJIVE-20 catalog is updated regularly, and the latest machine-readable version is available for download at http://safe.nrao.edu/vlba/mjivs/catalog.html.

Ref:=2014AJ....147...14D byDELLER A.T. , MIDDELBERG E. Astron. J., 147, 14 (2014) mJIVE-20: a survey for compact mJy radio objects with the Very Long Baseline Array. oTable 1: <MJV NNNNN> N=21396 among (Nos 00000-22207). =E=Catalogue in electronic form as <J/AJ/147/14/> Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   [MJV99]
   [MJV99] (Mantovani+Junor+Valerio+, 1999) (Not yet in Simbad) Write:<<[MJV99] 3C 273 N>> N: 5 Object:(Rad)  (SIMBAD class: Radio = Radio-source) Note:N=5 radio components of 3C 273. in source:3C 273 Ref:=1999NewAR..43..737M byMANTOVANI F. , JUNOR W., VALERIO C., McHARDY I. New Astronomy Reviews, 43, 737-740 (1999) Results of VLBI monitoring of 3C273 at 22 GHz and 43 GHz. oTables 1, 2: <[MJW99] 3C 273 N> (Nos 1-5). Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [MJZ20
   [MJZ20 . Not. R. Astron. Soc., 384, 1015-1033 (2008) The chemical compositions of 10 new sub-DLAs and strong Lyman-limit systems at z ≲ 1.5. oTable 2: <[MKL2008] QSO JHHMM+DDMM abs N.NNNN> N=10. Auth.:MEIRING J.D.+
Details on Acronym:   [MKL2014]
   [MKL2014] (Mao+Kong+Lin, 2014) (Not yet in Simbad) Write:<<[MKL2014] {NGC} NNNN-{UV|IR}NNN>> N: 400+343 Object:Cluster of *  (SIMBAD class: Cl* = Cluster of Stars) Note:N=400 UV clusters and N=343 IR clusters in four galaxies.
Use of SINGS and GALEX data. in source:M 81 = NGC 3031 in source:NGC 4536 in source:M 51 = NGC 5194 in source:NGC 7331 =E=Catalogue in electronic form as J/ApJ/789/76 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [MKM2002]
   [MKM2002] (Martini+Kelson+Mulchaev+, 2002)= (MKMT02) Write:<<[MKM2002] N>> N: 7 Object:AGN  (SIMBAD class: AGN = Active Galaxy Nucleus) Stat:is completely incorporated in Simbad Note:Chandra observations.
N=6 AGN members of ACO 2104 cluster + N=1 background AGN. in source:ACO 2104 Ref:=2002ApJ...576L.109M byMARTINI P. , KELSON D.D., MULCHAEY J.S., TRAGER S.C. Astrophys. J., 576, 109-112 (2002) An unexpectedly high fraction of active galactic nuclei in red cluster galaxies. oTable 1: <[MKM2002] N> (Nos 1-7). Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [MKM2003]
   [MKM2003] (Metcalfe+Kneib+McBreen+, 2003)= ([MKM2003a]) Write:<<[MKM2003] ISO ACO NNNN NNa>> N: 146 Object:IR G  (SIMBAD class: Galaxy) Stat:is completely incorporated in Simbad Note:ISO observations with ISOCAM through 3 lensing clusters of galaxies. in source:ACO 370 in source:ACO 2218 in source:ACO 2390 Ref:=2003A&A...407..791M byMETCALFE L. , KNEIB J.-P., McBREEN B., ALTIERI B., BIVIANO A., DELANEY M., ELBAZ D., KESSLER M.F., LEECH K., OKUMURA K., OTT S., PEREZ-MARTINEZ R., SANCHEZ-FERNANDEZ C., SCHULZ B. Astron. Astrophys., 407, 791-822 (2003) An ISOCAM survey through gravitationally lensing galaxy clusters. I. Source lists and source counts for A370, A2218 and A2390. oTable 2 : sources B NNN = LPS NNN. In reflist, Barvainis 1999 : ApJ is a misprint for AJ. oFigs 4, 5, Tables 4, 7: <[MKM2003] ISO ACO 370 NNa> (Nos 1-25, 11b-11c ). Figs 6, 7, Tables 5, 8: <[MKM 2003] ISO ACO 2218 NNa> N=68 among (Nos 2-75) + (Nos 15a-15b, 36a-36b, 61a-61b, 73a-73b). Figs 8, 9, Tables 6, 9: <[MKM2003] ISO A CO 2390 NNa> N=37 among (Nos 2-49) + (Nos 8a-8b, 28a-28b, 42a-42b). =E=Catalogue in electronic form as J/A+A/407/791 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [MKM2003a]
   [MKM2003a] (Metcalfe+Kneib+McBreen+, 2003) ***** Avoid the usage of [MKM2003a], prefer [MKM2003] Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [MKM2003b]
   [MKM2003b] (Movsessian+Khanzadyan+Magakian, 2003)= (CN) = (NIR) Write:<<[MKM2003b] CNNN>>
<<[MKM2003b] CNNW>> -129 (2004) The Giant Molecular Cloud associated with RCW 106. A 1.2 mm continuum mapping study. oTable 1: <[MKN2004] MMS NN> (Nos 1-95). Auth.:MOOKERJEA B.+ =E=Catalogue in electronic form as J/A+A/426/119 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [MKN2009]
   [MKN2009] (Matsunaga+Kawadu+Nishiyama+, 2009) Write:<<[MKN2009] NNNN>> N: 1364 Object:V*  (SIMBAD class: V* = Variable Star) Stat:is completely incorporated in Simbad Note:IRSF SIRIUS observations of N=1364 variable stars towards the Galactic Center. in source:NAME Galactic Center Ref:=2009MNRAS.399.1709M byMATSUNAGA N. , KAWADU T., NISHIYAMA S., NAGAYAMA T., HATANO H., TAMURA M., GLASS I.S., NAGATA T. Mon. Not. R. Astron. Soc., 399, 1709-1729 (2009) A near-infrared survey of Miras and the distance to the Galactic Centre. oTable 6: <[MKN2009] NNNN> (Nos 1-1364). Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [MKN2011]
   [MKN2011] (Matsunaga+Kawadu+Nishiyama+, 2011)= ([MKN2011a]) Write:<<[MKN2011] a>> N: 4 Object:Cepheid  (SIMBAD class: Cepheid = Cepheid variable Star) Stat:is completely incorporated in Simbad Note:IRSF SIRIUS observations of N=3 classical Cepheids in the nuclear bulge. Ref:=2011Natur.477..188M byMATSUNAGA N. , KAWADU T., NISHIYAMA S., NAGAYAMA T., KOBAYASHI N., TAMURA M., BONO G., FEAST M.W., NAGATA T. Natur, 477, 188-190 (2011) Three classical Cepheid variable stars in the nuclear bulge of the Milky Way. oFig. 1, Table 1: <[MKN2011] a> (Nos a-c). Ref:=2015ApJ...799...46M byMATSUNAGA N. , FUKUE K., YAMAMOTO R., KOBAYASHI N., INNO L., GENOVALI K., BONO G., BABA J., FUJII M.S., KONDO S., IKEDA Y., HAMANO S., NISHIYAMA S., NAGATA T., AOKI W., TSUJIMOTO T. Astrophys. J., 799, 46 (2015) Kinematics of classical cepheids in the nuclear stellar disk. oTable 1: <[MKN2011] a> (Nos d) added. Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [MKN2011a]
   [MKN2011a] (Matsunaga+Kawadu+Nishiyama+, 2011) ***** Avoid the usage of [MKN2011a], prefer [MKN2011] Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [MKN2011b]
   [MKN2011b] (Maeda+Kataoka+Nakamori+, 2011) Write:<<[MKN2011b] 1FGL JHHMM.m+DDMM>>
<<[MKN2011b] 1FGL JHHMM.m+DDMM src A>> N: 2+7 Object:(X)  (SIMBAD class: X = X-ray source) Stat:is completely incorporated in Simbad Note:Suzaku X-ray observations of four high Galactic latitude Fermi/LAT objects. Ref:=2011ApJ...729..103M byMAEDA K. , KATAOKA J., NAKAMORI T., STAWARZ L., MAKIYA R., TOTANI T., CHEUNG C.C., DONATO D., GEHRELS N., SAZ PARKINSON P., KANAI Y., KAWAI N., TANAKA Y., SATO R., TAKAHASHI T., TAKAHASHI Y. Astrophys. J., 729, 103 (2011) Unraveling the nature of unidentified high galactic latitude Fermi/LAT γ-ray sources with Suzaku. oTable 3: <[MKN2011b] 1FGL JHHMM.m+DDMM> N=2, <[MKN2011b] 1FGL JHHMM.m+DDMM src A> N=7. Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [MKO2006]
   [MKO2006] (Misawa+Kashikawa+Ohyama+, 2006) (Not yet in Simbad) Write:<<[MKO2006] QHHMM+DDd A>> N: 5 Object:Em. Obj.  (SIMBAD class: Em* = Emission-line Star) Note:UKIRT NIR survey for H-alpha emitting galaxies around the QSO Pair QSO 2343+125, QSO 2344+125.
See also [TMM98]. Ref:=2006AJ....131...34M byMISAWA T. , KASHIKAWA N., OHYAMA Y., HASHIMOTO T., IYE M. Astron. J., 131, 34-40 (2006) Near-infrared search for C IV absorption counterparts along the lines of sight to pair quasars. oTable 3, Figs 1, 2: <[MKO2006] Q2343+125 A> (Nos A-B), dImage = Gravitationally Lensed Image Note:Table 1, Fig.1: N=3 components of the gravitational lens system CLASS B1152+199 (Nos A-C).
See also [THB2000].
Table 2, Fig.5: N=6 components of the gravitational lens system CLASS B1359+154 (Nos A-F).
See also [RHN2000]. in source:CLASS B1152+199 in source:CLASS B1359+154 Ref:=1999AJ....117.2565M byMYERS S.T. , RUSIN D., FASSNACHT C.D., BLANDFORD R.D., PEARSON T.J. Astron. J., 117, 2565-2572 (1999) CLASS B1152+199 and B1359+154: two new gravitational lens systems discovered in the cosmic lens all-sky survey. oTable 1: <[MRF99] CLASS B1152+199 A> (Nos A-C). Table 2: <[MRF99] CLASS B1359+154 A> (Nos A-F). Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [MRG2000]
   [MRG2000] (Mould+Ridgewell+Gallagher+, 2000)= (Mould) Write:<<[MRG2000] RN>>
<<[MRG2000] NN>>
<<[MRG2000] Assoc N>> N: 8+81+6 Object:* + Assoc. of *  (SIMBAD class: Star) Note:Table 1: 2 brightest stars in each of the 4 chips. Table 2: Other stars in Cen A field. Fig.5: N=6 star associations. in source:Cen A = NGC 5128 Ref:=2000ApJ...536..266M byMOULD J.R. , RIDGEWELL A., GALLAGHER III J.S., BESSELL M.S., KELLER S., CALZETTI D., CLARKE J.T., TRAUGER J.T., GRILLMAIR C., BALLESTER G.E., BURROWS C.J., KRIST J., CRISP D., EVANS R., GRIFFITHS R., HESTER J.J., HOESSEL J.G., HOLTZMAN J.A., SCOWEN P.A., STAPELFELDT K.R., SAHAI R., WATSON A., MEADOWS V. Astrophys. J., 536, 266-276 (2000) Jet-induced star formation in Centaurus A. oGraham's stars are [FG2000b] NN in SIMBAD. oTable 1: <[MRG2000] RN> (Nos R1-R8). Table 2: <[MRG2000] NN> (Nos 1-81). Fig.5: <[MRG2000] Assoc N> (Nos 1-6). Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [MRG2005]
   [MRG2005] (Muxlow+Richards+Garrington+, 2005) Write:<<[MRG2005] JHHMMSS+DDMMSS>> N: 92 Object:(Rad)  (SIMBAD class: Radio = Radio-source) Note:MERLIN and VLA data of the HDF and flanking fields. in source:NAME HDFN Ref:=2005MNRAS.358.1159M byMUXLOW T.W.B. , RICHARDS A.M.S., GARRINGTON S.T., WILKINSON P.N., ANDERSON B., RICHARDS E.A., AXON D.J., FOMALONT E.B., KELLERMANN K.I., PARTRIDGE R.B., WINDHORST R.A. Mon. Not. R. Astron. Soc., 358, 1159-1194 (2005) High-resolution studies of radio sources in the Hubble Deep and flanking fields. oPhase calibration source which lies less than 40arcmin from the HDF centre (J124129+622041) is not identified. References: CBHCS04 = 2004AJ....127.3137C (not ApJ), H01 = 2001ApJ...554..742H (not AJ), D02 = 2001AJ....122..598D (not 2002). oTables A1, A2: <[MRG2005] JHHMMSS+DDMMSS> N=92. =E=Catalogue in electronic form as J/MNRAS/358/1159 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [MRH2010]
   [MRH2010] (Magids+Rigopoulou+Huang+, 2010) (Not yet in Simbad) Write:<<[MRH2010] CNN-Q1700>>
<<[MRH2010] DNN-Q1700>> N: 5+5 Object:G  (SIMBAD class: Galaxy) Note:N=10 Lyman Break Galaxies at z∼3, using Spitzer IRAC observations. Ref:=2010MNRAS.401.1521M byMAGDIS G.E. , RIGOPOULOU D., HUANG J.-S., FAZIO G.G. Mon. Not. R. Astron. Soc., 401, 1521-1531 (2010) On the stellar masses of IRAC detected Lyman break galaxies at z ~ 3. oTables 1-2: <[MRH2010] CNN-Q1700> N=5, <[MRH2010] DNN-Q1700> N=5. =E=Catalogue in electronic form as J/MNRAS/401/1521 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [MRH2014]
   [MRH2014] (Magdis+Rigopoulou+Hopwood+, 2014) Write:<<[MRH2014] BOOTESN>>
<<[MRH2014] CDFSN>>
<<[MRH2014] ELAISA>>
<<[MRH2014] FLSNN>>
<<[MRH2014] SWIREN>>
<<[MRH2014] HLSW-NN>>
<<[MRH2014] XMMN>> N: 18 Object:ULIRG  (SIMBAD class: Galaxy) Stat:is completely incorporated in Simbad Note:Spitzer and Herschel IR observations of N=17 ultra-luminous infrared galaxies in the redshift range 0.12 ≤z≤ 0.88. Ref:=2014ApJ...796...63M byMAGDIS G.E. , RIGOPOULOU D., HOPWOOD R., HUANG J.-S., FARRAH D., PEARSON C., ALONSO-HERRERO A., BOCK J.J., CLEMENTS D., COORAY A., GRIFFIN M.J., OLIVER S., PEREZ FOURNON I., RIECHERS D., SWINYARD B.M., SCOTT D., THATTE N., VALTCHANOV I., VACCARI M. Astrophys. J., 796, 63 (2014) A far-infrared spectroscopic survey of intermediate redshift (ultra) luminous infrared galaxies. oTables 1-4: <[MRH2014] BOOTESN> N=3, <[MRH2014] CDFSN> N=2, <[MRH2014] ELAISA> N=2, <[MRH2014] FLS0N> N=2, <[MRH2014] SWIREN> N=6 among (Nos SWIRE1-SWIRE7), <[MRH2014] HLS-NN> N=1, <[MRH2014] XMMN> N=2. Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [MRH89]
   [MRH89] (Meisenheimer+Roser+Hiltner+, 1989) Write:<<[MRH89] 3C NNN W>> N: 7 Object:(Rad)  (SIMBAD class: Radio = Radio-source) Stat:is completely incorporated in Simbad Note:Hotspots in 3C objects. in source:3C 20 in source:3C 65 in source:3C 111 in source:3C 123 in source:3C 303 Ref:=1989A&A...219...63M byMEISENHEIMER K. , ROESER H.-J., HILTNER P.R., YATES M.G., LONGAIR M.S., CHINI R., PERLEY R.A. Astron. Astrophys., 219, 63-86 (1989)


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