Table A.1.
Gaussian fits to the log SSFR distribution.
| Type | μSF | σSF | μQ | σQ | T | N |
|---|---|---|---|---|---|---|
| z1 = [0.01, 0.1] | ||||||
| Field | –10.0 | 0.4 | –11.5 | 0.7 | –10.7 | 3981 |
| Central | –10.3 | 0.5 | –12.1 | 0.5 | –11.1 | 762 |
| Satellite | –10.2 | 0.5 | –11.8 | 0.5 | –11.0 | 2146 |
| z2 = [0.1, 0.2] | ||||||
| Field | –10.3 | 0.4 | –11.6 | 0.4 | –10.9 | 8500 |
| Central | –10.4 | 0.5 | –11.9 | 0.4 | –11.1 | 2232 |
| Satellite | –10.6 | 0.5 | –11.7 | 0.4 | –11.1 | 4250 |
| z3 = [0.2, 0.3] | ||||||
| Field | –10.5 | 0.4 | –11.5 | 0.3 | –11.0 | 7037 |
| Central | –10.8 | 0.6 | –11.7 | 0.3 | –11.2 | 1972 |
| Satellite | –10.8 | 0.5 | –11.6 | 0.3 | –11.2 | 2806 |
Notes. The columns are: galaxy type; location and scale parameter of the star-forming Gaussian, μSF (in unit of Gyr−1) and σSF (in dex); location and scale parameter of the quiescent Gaussian, μQ (in unit of Gyr−1) and σQ (in dex); threshold T (in unit of Gyr−1) in log SSFR where the amplitudes of two Gaussians are equal to each other, and number of galaxies.
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