Table 4
Final sample used in the analysis.
| z |  |
NG&C | Ngals in G&C | Ngals in the field | ||||
|---|---|---|---|---|---|---|---|---|
 |
 |
 |
 |
|||||
| all | < 1043 erg/s | > 1043 erg/s | all | < 1043 erg/s | > 1043 erg/s | |||
| 0.1–0.2 | 9.6 | 21 | 16 | 5 | 920 (1116) | 420 (530) | 500 (586) | 4402 (6098) |
| 0.2–0.3 | 10.4 | 34 | 17 | 17 | 502 (751) | 182 (272) | 320 (479) | 4654 (6729) |
| 0.3–0.4 | 10.8 | 24 | 11 | 13 | 187 (351) | 85 (135) | 102 (216) | 2468 (4009) |
| 0.4–0.6 | 11.0 | 38 | – | – | 141 (531) | – | – | 2595 (13 188) |
| Total | 117 | 44 | 35 | 1746 (3132) | 687 (937) | 922 (1281) | 14 119 (30 024) | |
Notes. Numbers are given according to the four redshift bins given in Col. 1. Column 2 gives the stellar mass limit. Columns 3−5 indicate the total number of G&C, and the number of G&C in the two luminosity bins in which the GSMF has been studied, which contain galaxies with stellar masses above the mass limit. The remaining columns indicate the number of galaxies above the stellar mass limit in G&C, divided again into luminosity classes, and the number of galaxies in the corresponding field sample; the quantities in parentheses refer to the number of galaxies weighted for spectroscopic completeness.
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