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Table 1
Samples of passive galaxies with relative morphological compositions, selected using different sSFR thresholds, according to the different IMFs adopted in the population synthesis models.
IMF type | sSFR threshold | Passive | ETGs | LTGs |
[yr-1] | galaxies | fraction | fraction | |
|
||||
Salpeter | ≤ 1.0 × 10-11 | 281 | 182 | 99 |
Chabrier | ≤ 1.2 × 10-11 | 295 | 184 | 111 |
s = 1.5 | ≤ 5.7 × 10-12 | 319 | 181 | 138 |
s = 2.0 | ≤ 7.7 × 10-12 | 313 | 193 | 120 |
s = 2.5 | ≤ 1.4 × 10-11 | 283 | 182 | 101 |
s = 3.0 | ≤ 3.1 × 10-11 | 280 | 179 | 101 |
s = 3.5 | ≤ 7.1 × 10-11 | 286 | 182 | 104 |
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