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 |
by | CANAMERAS 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) | |
Planck's dusty GEMS: The brightest gravitationally lensed galaxies discovered with the Planck all-sky survey. | |
o | Table 1: <[CNG2015] PLCK GLLL.l+BB.b> N=11. |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |