A deeper view of extremely red galaxies: the redshift distribution in the GOODS/CDFS ISAAC field
A deeper view of extremely red galaxies: the redshift distribution in the GOODS/CDFS ISAAC field
复制标题
更深入地观察极红星系:GOODS/CDFS ISAAC 场中的红移分布
DOI:
10.1111/j.1365-2966.2004.08044.x
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发表时间:
2004
影响因子:
4.8
通讯作者:
Nathan D. Roche
中科院分区:
文献类型:
--
作者:
K. Caputi;J. Dunlop;R. McLure;Nathan D. Roche
We have analysed five-epoch Great Observatories Origins Deep Survey (GOODS) HST-ACS B, V, I-775 and z data sets (v. 1.0 release), in conjunction with existing VLT-ISAAC imaging in the J, H and K-s bands, to derive estimated redshifts for the sample of 198 extremely red galaxies (ERGs) with K-s 3.92 selected by Roche, Dunlop & Almaini (2003) from 50.4 arcmin(2) of the GOODS/Chandra Deep Field South. We find that, at this depth, the ERG population spans the redshift range 0.5 L population at redshifts zphot > 2. We determine lower limits of c = (6.1 +/- 1.9) x 10(-5) Mpc(-3) and rho(c) = (2.1 +/- 1.1) x 10(-5) Mpc(-3) on the comoving densities of progenitors of local massive galaxies already assembled at redshifts zphot = 2.5 and zphot = 3.5, respectively. We have investigated the existence of high-redshift Lyman-break galaxies massive enough to be included in this ERG sample. Out of an initial list of 12 potential very high redshift candidates, we have identified two ERGs which have a high probability of lying at z(phot) > 4. We discuss the advantages of multicolour to single-colour selection techniques in obtaining reliable lists of very high redshift candidate sources, and present revised lower redshift estimates for sources previously claimed as potential z > 5 dropouts in recent studies.
影响因子:
4.9
作者:
Charlot, S;Fall, SM
通讯作者:
Fall, SM