Details on Acronym: [CNL2018] | |
| [CNL2018] | (Canameras+Nesvadba+Limousin+, 2018) |
| Write: | <<[CNL2018] PLCK G165.7+67.0 system>> <<[CNL2018] PLCK G165.7+67.0 lens>> <<[CNL2018] PLCK G165.7+67.0 N.N>> <<[CNL2018] PLCK G165.7+67.0 Co-W>> |
| N: | 1+1+24+2 |
| Object: | Grav. lens system + Grav. lens + Grav. lensed image (SIMBAD class: Unknown = Object of Unknown Nature) |
| Stat: | is completely incorporated in Simbad |
| Note: | HST WFC3, CFHT Megacam and WIRCAM, Spitzer IRAC, SMA and PdBI observations of N=1 gravitational lens, N=24+2 gravitationally lensed images of the background galaxy [CNG2015] PLCK G165.7+67.0, forming N=1 gravitational lens system. See also [CNK2017]. |
| Ref: | =2018A&A...620A..60C |
| by | CANAMERAS R. , NESVADBA N.P.H., LIMOUSIN M., DOLE H., KNEISSL R., KOENIG S., LE FLOC'H E., PETITPAS G., SCOTT D. |
| Astron. Astrophys., 620A, 60-60 (2018) | |
| Planck's dusty GEMS. V. Molecular wind and clump stability in a strongly lensed star-forming galaxy at z = 2.2. | |
| o | <[CNL2018] PLCK G165.7+67.0 system> N=1. <[CNL2018] PLCK G165.7+67.0 lens> N=1. Fig. 5, Table 3: <[CNL2018] PLCK G165.7+67.0 N.N>, N=24 among (Nos 1.1-1.2 to 9.1-9.2). Figs 5+11, Table 6: <[CNL2018] PLCK G165.7+67.0 Co-W> (Nos Co-N, Co-S). |
| o | PLCK G165.7+49.0 is a misprint for [CNG2015] PLCK G165.7+67.0 |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |