Table 9.
Values ρ0 and γ that best fit our co-moving number density calculation (see Eq. (13)) of green valley galaxies at different stellar mass bins and SSP models.
| BC03 |
EMILES+BaSTI |
EMILES+Padova00 |
||||
|---|---|---|---|---|---|---|
| log10 ρ0 | γ | log10 ρ0 | γ | log10 ρ0 | γ | |
| 10.0 ≤ log10 M⋆ < 10.4 |
 |
 |
 |
 |
 |
 |
| 10.4 ≤ log10 M⋆ < 10.8 |
 |
 |
 |
 |
 |
 |
| 10.8 ≤ log10 M⋆ < 11.2 |
 |
 |
 |
 |
 |
 |
| log10 M⋆ ≥ 11.2 |
 |
 |
 |
 |
 |
 |
Notes. There are no ρ0 and γ fitting values for the lowest stellar mass bin, 9.6 ≤ log10 M⋆ < 10, because this subsample is only available at the lowest redshift bin, 0.1 ≤ z < 0.3. All the values were obtained at setting h = 1.
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