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

Result of query: info cati CNG2015] PLCK$



.
 
 lignment in two radio galaxies at z ~ 2 with extended light    profiles: Similarities to brightest cluster galaxies.
oTable 2: <[CND2015] a> N=7 (Nos a-g).
 Auth.:COLLET C.+

Details on Acronym:   [CNG2015]
   [CNG2015] (Canameras+Nesvadba+Guery+, 2015) Write:<<[CNG2015] PLCK GLLL.l+BB.b>> N: 11 Object:Grav. lensed image of a G  (SIMBAD class: LensedG = Gravitationally Lensed Image of a Galaxy) Stat:is completely incorporated in Simbad Note:IRAM 30m telescope EMIR CO line observations of N=11 bright far-infrared (FIR) and sub-mm sources discovered through a combination of the Planck all-sky survey and follow-up Herschel-SPIRE imaging, also known as "Planck’s Dusty GEMS (Gravitationally Enhanced subMillimetre Sources)".
Use of SDSS data. Ref:=2015A&A...581A.105C byCANAMERAS R. , NESVADBA N.P.H., GUERY D., McKENZIE T., KOENIG S., PETITPAS G., DOLE H., FRYE B., FLORES-CACHO I., MONTIER L., NEGRELLO M., BEELEN A., BOONE F., DICKEN D., LAGACHE G., LE FLOC'H E., ALTIERI B., BETHERMIN M., CHARY R., DE ZOTTI G., GIARD M., KNEISSL R., KRIPS M., MALHOTRA S., MARTINACHE C., OMONT A., POINTECOUTEAU E., PUGET J.-L., SCOTT D., SOUCAIL G., VALTCHANOV I., WELIKALA N., YAN L. Astron. Astrophys., 581A, 105-105 (2015)

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