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

Result of query: info cati GPSR$
 1 (2004)
    A search for shock-excited molecular hydrogen knots in Chamaeleon I
    very low mass YSOs.
oTable 2: <[GPM2004] AN> (Nos A-D, B1-B2, C1-C3).
 Auth.:GOMEZ M.+

Details on Acronym:   [GPM2009]
   [GPM2009] (Guseva+Papaderos+Meyer+, 2009) Write:<<[GPM2009] JHHMM+DDMM N>>
<<[GPM2009] JHHMM+DDMM BGN>>
<<[GPM2009] NNNNNN>>
<<[GPM2009] GHHMMSSs+DDMMSS N>>
<<[GPM2009] GHHMMSSs+DDMMSS BG>>
<<[GPM2009] HHMM+DDMM>>
<<[GPM2009] PHL293B>> N: 38+28 Object:EmG  (SIMBAD class: EmG = Emission-line galaxy) Stat:is completely incorporated in Simbad Note:VLT FORS2 and ESO 3.6m telescope EFOSC2 spectroscopy of HII regions in emission-line galaxies. Ref:=2009A&A...505...63G byGUSEVA N.G. , PAPADEROS P., MEYER H.T., IZOTOV Y.I., FRICKE K.J. Astron. Astrophys., 505, 63-72 (2009) An investigation of the luminosity-metallicity relation for a large sample of low-metallicity emission-line galaxies. oTables 1, 2: <[GPM2009] JHHMM+DDMM N>, <[GPM2009] JHHMM+DDMM {BG}N>, <[GPM2009] NNNNNN>, <[GPM2009] GHHMMSSs+DDMMSS N>, <[GPM2009] GHHMMSSs+DDMMSS {BG}>, <[GPM20 LEY R.A. Astrophys. J., Suppl. Ser., 74, 181-224 (1990) A catalog of small-diameter radio sources in the galactic plane. oTable 4: <GPSR LLL.lll+BB.bbb> N=1992 Ref:=1992ApJS...80..211H byHELFAND D.J. , ZOONEMATKERMANI S., BECKER R.H., WHITE R.L. Astrophys. J., Suppl. Ser., 80, 211-255 (1992) Compact radio sources near the galactic plane. oTable 3: <GPSR LLL.lll+BB.bbb> N=1457 Ref:=1994ApJS...91..347B byBECKER R.H. , WHITE R.L., HELFAND D.J., ZOONEMATKERMANI S. Astrophys. J., Suppl. Ser., 91, 347-387 (1994) A 5GHz VLA survey of the galactic plane. oTable 2: <GPSR5 LLL.lll+B.bbb> N=1272, <GPSR LLL.lll+B.bbb> N=5 =E=Catalogue in electronic form as J/ApJS/74/181 =E=Catalogue in electronic form as <J/ApJS/80/211/> Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   GPS
   GPS (Gal. Plane Survey) ***** Avoid the usage of GPS, prefer GPSR5 Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   [GPS2005]
   [GPS2005] (Gorosabel+Perez-Ramirez+Sollerman+, 2005) Write:<<[GPS2005] JHHMMSS.ss+DDMMSS.s>> N: 1 Originof the Acronym: S = Created by Simbad, the CDS Database Object:G  (SIMBAD class: Galaxy) Stat:is completely incorporated in Simbad Note:VLT FORS observations of a galaxy near the host galaxy of GRB 030329. Ref:=2005A&A...444..711G byGOROSABEL J. , PEREZ-RAMIREZ D., SOLLERMAN J., DE UGARTE POSTIGO A., FYNBO J.P.U., CASTRO-TIRADO A.J., JAKOBSSON P., CHRISTENSEN L., HJORTH J., JOHANNESSON G., GUZIY S., CASTRO CERON J.M., BJOERNSSON G., SOKOLOV V.V., FATKHULLIN T.A., NILSSON K. Astron. Astrophys., 444, 711-721 (2005) The GRB 030329 host: a blue low metallicity subluminous galaxy with intense star formation. oThe host galaxy of GRB 030329 = [GPE2003] GRB 030329 abs 0.1685 oParagr. 3.6: <[GPS2005] JHHMMSS.ss+DDMMSS.s> N=1.
Details on Acronym:   [GPS2008]
   [GPS2008] (Greve+Pope+Scott+, 2008)= (GN) = (MM) Write:<<[GPS2008] MM JHHMMSS+DDMMSS>>
<<[GPS2008] GN 1200.NN>> N: 47 Object:G  (SIMBAD class: Galaxy) Stat:is completely incorporated in Simbad Note:IRAM 30m MAMBO 1200mu.m observations of the GOODS North Field. in source:NAME GOODS North Field Ref:=2008MNRAS.389.1489G byGREVE T.R. , POPE A., SCOTT D., IVISON R.J., BORYS C., CONSELICE C.J., BERTOLDI F. Mon. Not. R. Astron. Soc., 389, 1489-1506 (2008) A 1200-µm MAMBO survey of the GO ionally Lensed Image Note:Potential arcs, lensed images of LCDCS 280, 480, 954. Ref:=2003ApJ...584..691Z byZARITSKY D. , GONZALEZ A.H. Astrophys. J., 584, 691-701 (2003) On the incidence of strong gravitational lensing by clusters in the Las Campanas distant cluster survey. oFigs 3-5, Table 2: <[ZG2003] LCDCS 280 N> (Nos 1-6), <[ZG2003] LCDCS 480 Na> (Nos 1, 1a-1b), <[ZG2003] LCDCS 954 N> (Nos 1-4). Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [ZG98]
   [ZG98] (Zhao+Goss, 1998) (Not yet in Simbad) Write:<<[ZG98] NN>>
<<[ZG98] NN-A>> N: 12+25 Object:HII  (SIMBAD class: HII = HII (ionized) region) Note:Fig.1a: (N

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