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

Result of query: info cati MML2015] 5BZU$



.
 
 OTTHELF E.V.
 Astrophys. J., 551, 1016-1023 (2001)

    3EG J2016+3657: confirming an EGRET blazar behind the galactic plane.

o(Erratum) erratum vol. 572, p. 693 (2002)
oTable 1: <[MGH2000] NN> (Nos 15-19) added.
 Auth.:HALPERN J.P.+

Details on Acronym:   [MGH2008]
   [MGH2008] (McIntosh+Guo+Hertzberg+, 2008) Write:<<[MGH2008] Group NNNN>>
<<[MGH2008] JHHMMSS.s+DDMMSS.s>>
<<[MGH2008] NYU NNNNNN>> N: 38+83 Object:Group of G + G in Pair  (SIMBAD class: Galaxy) Note:Archival SDSS images are used to search for pairs of massive galaxies merging in dense group and cluster environments. Ref:=2008MNRAS.388.1537M byMcINTOSH D.H. , GUO Y., HERTZBERG J., KATZ N., MO H.J., VAN DEN BOSCH F.C., YANG X. Mon. Not. R. Astron. Soc., 388, 1537-1556 (2008) Ongoing assembly of massive galaxies by major merging in large groups and clusters from the SDSS. oTables 2, 3, col(1): <[MGH2008] Group NNNN> N=38. Tables 2, 3, col(4), Fig.3: <[MGH2008] NYU NNNNNN> N=35 = Tables 2, 3, cols(5,6): <[MGH2008]JHHMMSS.s+DDMMSS.s> N=76. =E=Catalogue in electronic form as J/MNRAS/388/1537 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [MGH2009]
   [MGH2009] (Mukherjee+Gotthelf+Halpern, 2009) Write:<<[MGH2009] NN>> N: 16 Object:(X)  (SIMBAD class: X = X-ray source) Stat:is completely incorporated in Simbad Note:XMM-Newton observations of the field around HESS J1834-087. Ref:=2009ApJ...691.1707M byMUKHERJEE R. , GOTTHELF E.V., HALPERN J.P. Astrophys. J., 691, 1707-1711 (2009) On the origin of TeV γ-ray emission from HESS J1834-087. oTable 1, Fig.1: <[MGH2009] NN> (Nos 1-16). Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   [MGH2
   [MGH2 = [WSL93] 3 Auth.:MISGELD I.+ =E=Catalogue in electronic form as J/A+A/531/A4
Details on Acronym:   [MMJ2002]
   [MMJ2002] (Magliocchetti+Maddox+Jackson+, 2002) Write:<<[MMJ2002] NNNNNN>> N: 557+270 Object:rG  (SIMBAD class: RadioG = Radio Galaxy) Note:The authors have used the 2dFGRS and the APM data to study properties of radio-sources from the FIRST survey. Ref:=2002MNRAS.333..100M byMAGLIOCCHETTI M. , MADDOX S.J., JACKSON C.A., BLAND-HAWTHORN J., BRIDGES T., CANNON R., COLE S., COLLESS M., COLLINS C., COUCH W., DALTON G., DE PROPRIS R., DRIVER S.P., EFSTATHIOU G., ELLIS R.S., FRENK C.S., GLAZEBROOK K., LAHAV O., LEWIS I., LUMSDEN S., PEACOCK J.A., PETERSON B.A., SUTHERLAND W., TAYLOR K. Mon. Not. R. Astron. Soc., 333, 100-120 (2002) The 2dF Galaxy Redshift Survey: the population of nearby radio galaxies at the 1-mJy level. oTables 2, 3: <[MMJ2002] NNNNNN> N=557 among (Nos 266022-332679). Ref:=2004MNRAS.350.1485M byMAGLIOCCHETTI M. , MADDOX S.J., HAWKINS E., PEACOCK J.A., BLAND-HAWTHORN J., BRIDGES T., CANNON R., COLE S., COLLESS M., COLLINS C., COUCH W., DALTON G., DE PROPRIS R., DRIVER S.P., EFSTATHIOU G., ELLIS R.S., FRENK C.S., GLAZEBROOK K., JACKSON C.A

© Université de Strasbourg/CNRS

    • Contact