Table 3.
Description of the galaxy samples.
| log10(M*/M⊙) |
M*, med/M⊙ | log(M200m, CEN/M⊙) |
Redshift |
FULLspec | CEN | SAT | |||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| min | max | 16% | med | 84% | min | max | med | Ng | Ng | Ng | |
| 10.0 | 10.5 | 1.8 × 1010 | 11.5 | 11.75 | 12.1 | 0.01 | 0.06 | 0.05 | 11922 | 7956 | 3966 |
| 10.5 | 11.0 | 5.5 × 1010 | 11.8 | 12.1 | 12.6 | 0.02 | 0.10 | 0.08 | 45248 | 30825 | 14423 |
| 11.0 | 11.25 | 1.3 × 1011 | 12.2 | 12.7 | 13.1 | 0.02 | 0.15 | 0.12 | 34046 | 26099 | 7947 |
| 11.25 | 11.5 | 2.2 × 1011 | 12.6 | 13.1 | 13.6 | 0.03 | 0.19 | 0.15 | 24098 | 20342 | 3756 |
| log10(M200m/M⊙) |
M200m, med/M⊙ | log(M*, CENhalo/M⊙) |
Redshift |
CENhalo | SAThalo | ||||||
| min | max | 16% | med | 84% | min | max | med | Ng | Ng | ||
| 11.5 | 12.0 | 5.5 × 1011 | 9.7 | 10.2 | 10.6 | 0.01 | 0.08 | 0.06 | 25368 | 903 | |
| 12.0 | 12.5 | 1.7 × 1012 | 10.4 | 10.7 | 11.0 | 0.02 | 0.13 | 0.09 | 41301 | 4140 | |
| 12.5 | 13.0 | 5.0 × 1012 | 10.8 | 11.0 | 11.2 | 0.02 | 0.16 | 0.12 | 30740 | 9145 | |
| 13.0 | 13.5 | 1.6 × 1013 | 11.1 | 11.25 | 11.4 | 0.03 | 0.20 | 0.14 | 19889 | 9785 | |
| 13.5 | 14.0 | 4.8 × 1013 | 11.2 | 11.4 | 11.6 | 0.03 | 0.20 | 0.16 | 8214 | 12537 | |
| log10(M*/M⊙) |
M*, med/M⊙ | Redshift |
FULLphot | Isolated | |||||||
| min | max | min | max | med | Ng | Ng | |||||
| 9.5 | 10.0 | 5.5 × 109 | 0.01 | 0.09 | 0.07 | 95698 | 24280 | ||||
| 10.0 | 10.5 | 1.8 × 1010 | 0.01 | 0.12 | 0.10 | 214286 | 50137 | ||||
| 10.5 | 11.0 | 5.5 × 1010 | 0.02 | 0.17 | 0.14 | 415627 | 70348 | ||||
| 11.0 | 11.25 | 1.3 × 1011 | 0.02 | 0.33 | 0.28 | 627757 | 50766 | ||||
| 11.25 | 11.5 | 2.2 × 1011 | 0.03 | 0.40 | 0.35 | 324541 | 17983 | ||||
Notes. For each table, from left to right, the columns are the stellar (halo) mass bin, median stellar (halo) mass, 16th percentile, median, and 84th percentile halo (stellar) mass of central galaxies, redshift bin, median redshift, and number of galaxies in the sample. Top: The FULLspec, CEN, and SAT galaxy samples built from SDSS MGS. FULLspec contains all galaxies within the stellar mass bin and redshift bin. We split the FULLspec sample into central (CEN) or satellite (SAT) galaxy samples according to the group finder algorithm (Tinker 2021). Middle: The CENhalo and SAThalo sample of central galaxies binned in halo mass, built from SDSS MGS and is based on the group finder algorithm (Tinker 2021). Bottom: The FULLphot and isolated galaxy samples built from DESI LS DR9. The FULLphot contains all galaxies within the stellar mass bin and redshift bin. We select the isolated sample with the algorithm defined in Appendix. D.
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