Details on Acronym: BzK | |
| BzK | (B, z, and K-band photometry) |
| ***** | Avoid the usage of BzK, prefer [LSE2007] |
| Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: DRG | |
| DRG | (Distant Red Galaxy) |
| ***** | Avoid the usage of DRG, prefer [LSE2007] |
| Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: [LSE2007] | |
| [LSE2007] | (Law+Steidel+Erb+, 2007)= (BzK) = (DRG) = (SMG) |
| Write: | <<[LSE2007] BzKNNN>> <<[LSE2007] DRGNN>> <<[LSE2007] SMGNN>> |
| N: | 13+13+4 |
| Object: | G (SIMBAD class: Galaxy) |
| Stat: | is completely incorporated in Simbad |
| Note: | Use of archival HST ACS data. Morphology of z about 2-3 galaxies: In the format BzK stands for B, z, and K-band photometry, DRG stands for Distant Red Galaxies, SMG for SubMillimeter Galaxies. See also [RSE2006]. |
| in source: | NAME GOODS North Field |
| Ref: | =2007ApJ...656....1L |
| by | LAW D.R. , STEIDEL C.C., ERB D.K., PETTINI M., REDDY N.A., SHAPLEY A.E., ADELBERGER K.L., SIMENC D.J. |
| Astrophys. J., 656, 1-26 (2007) | |
| The physical nature of rest-UV galaxy morphology during the peak epoch of galaxy formation. | |
| o | Figs 19, 21, 22: <[LSE2007] BzKNNN> N=13 among (Nos BzK3 to BzK451), <[LSE2007] DRGNN> N=13 among (Nos DRG1 to DRG71), <[LSE2007] SMGNN> N=4 among (Nos SMG4 to SMG13). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |
Details on Acronym: SMG | |
| SMG | (SubMillimeter Galaxy) |
| ***** | Avoid the usage of SMG, prefer [LSE2007] |
| Origin | of the Acronym: A = Assigned by the author(s) |