Table 2.
Characteristics of the spectroscopic redshift samples.
| COSMOS Spectroscopic surveys | Nb | zmed | zrange |
 |
References |
|---|---|---|---|---|---|
| zCOSMOS-bright VIMOS / VLT | 8608 | 0.48 | [0.02, 1.19] | 21.6 | (1) |
| FORS2/VLT | 788 | 0.89 | [0.07, 3.65] | 22.6 | (2) |
| DEIMOS/Keck II | 2022 | 0.93 | [0.02, 5.87] | 23.2 | (3, 4) |
| FMOS/Subaru | 26 | 1.21 | [0.82, 1.50] | 22.5 | (5) |
| MOIRC/Subaru | 10 | 1.41 | [1.24, 2.09] | 23.9 | (6) |
| FMOS/Subaru | 178 | 1.56 | [1.34, 1.73] | 23.5 | (7) |
| WFC3-grism HST | 11 | 2.03 | [1.88, 2.54] | 25.1 | (8) |
| zCOSMOS deep VIMOS/VLT | 767 | 2.11 | [1.50, 2.50] | 23.8 | (9) |
| MOSDEF MOSFIRE/Keck I | 80 | 2.15 | [0.80, 3.71] | 24.2 | (10) |
| XSHOOTER/VLT | 14 | 2.19 | [1.98, 2.48] | 22.2 | (11, 12) |
| VUDS VIMOS/VLT | 998 | 2.70 | [0.10, 4.93] | 24.6 | (13) |
| DEIMOS 10K DEIMOS/Keck II | 6617 | 1 & 4 | [0.00, 6.00] | 23 | (14) |
Notes. Only the most secure spectroscopic redshifts (those with a flag between three and four) were considered. The redshift range, median redshift, and apparent magnitude in the band are provided for each selected sample. (1) Lilly et al. (2007); (2) Comparat et al. (2015); (3) Capak et al. (in prep.); (4) Kartaltepe et al. (2010); (5) Roseboom et al. (2012); (6) Onodera et al. (2012); (7) Silverman et al. (2015); (8) Krogager et al. (2014); (9) Lilly et al. (2016, in prep.); (10) Kriek et al. (2015); (11) Stockmann et al. (in prep.); (12) Zabl (2015); (13) Le Fèvre et al. (2015); (14) Hasinger et al. (2018).
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