Table 1.
Galaxy samples used in this work.
| log10(M*/M⊙) | redshift | Ngal | |||
|---|---|---|---|---|---|
| min | max | min | max | CENSF | CENQU |
| 10.0 | 10.5 | 0.01 | 0.06 | 5226 | 2516 |
| 10.5 | 11.0 | 0.02 | 0.10 | 13 668 | 16 485 |
| 11.0 | 11.25 | 0.02 | 0.15 | 8070 | 17 466 |
| 11.25 | 11.5 | 0.03 | 0.19 | 4279 | 15 663 |
| log10(M200 m/M⊙) | redshift | Ngal | |||
| min | max | min | max | CENhalo, SF | CENhalo, QU |
| 11.5 | 12.0 | 0.01 | 0.08 | 20 206 | 5162 |
| 12.0 | 12.5 | 0.02 | 0.13 | 29 791 | 11 510 |
| 12.5 | 13.0 | 0.02 | 0.16 | 12 103 | 18 637 |
| 13.0 | 13.5 | 0.03 | 0.20 | 1788 | 18 101 |
| 13.5 | 14.0 | 0.03 | 0.20 | – | 8209 |
Notes. Top: Central star-forming (CENSF) and quiescent (CENQU) galaxy samples binned in stellar masses. From left to right, the columns are the stellar mass bin, redshift bin and number of star-forming (or quiescent) galaxies in the sample. Bottom: Central star-forming (CENhalo, SF) and quiescent galaxies (CENhalo, QU) binned in halo mass. From left to right, the columns are the halo mass bin, redshift bin, and the number of star-forming (or quiescent) galaxies in the sample.
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