Table A.6.
Same as Table A.1, but for probability distribution functions of extinctions (see Eq. (A.4)).
| AV | Ngal | μAV |
 |
|||
|---|---|---|---|---|---|---|
| μ1 | μ0 | σ1 | σ0 | |||
| 10.0 ≤ log10 M⋆ < 10.4 | 1429 |
 |
 |
 |
 |
|
| BC03 | 10.4 ≤ log10 M⋆ < 10.8 | 2526 |
 |
 |
 |
 |
| 10.8 ≤ log10 M⋆ < 11.2 | 3181 |
 |
 |
 |
 |
|
| ( * )log10 M⋆ ≥ 11.2 | 1122 |
 |
 |
 |
 |
|
| 10.1 ≤ log10 M⋆ < 10.5 | 1284 |
 |
 |
 |
 |
|
| EMILES+BaSTI | 10.5 ≤ log10 M⋆ < 10.9 | 2370 |
 |
 |
 |
 |
| 10.9 ≤ log10 M⋆ < 11.3 | 3089 |
 |
 |
 |
 |
|
| log10 M⋆ ≥ 11.3 | 1159 |
 |
 |
 |
 |
|
| 10.1 ≤ log10 M⋆ < 10.5 | 1329 |
 |
 |
 |
 |
|
| EMILES+Padova00 | 10.5 ≤ log10 M⋆ < 10.9 | 2335 |
 |
 |
 |
 |
| 10.9 ≤ log10 M⋆ < 11.3 | 2945 |
 |
 |
 |
 |
|
| log10 M⋆ ≥ 11.3 | 1141 |
 |
 |
 |
 |
|
Notes.( * )For quiescent galaxies and BC03 SSP models at 0.1 ≤ z < 0.2 and log10 M⋆ ≥ 11.2, the assumption of linear dependence for σint(z) and μ(z) is too strict, and we imposed σint(0.1 ≤ z < 0.2)=σint(z = 0.2) = 0.14 ± 0.03 and μ(0.1 ≤ z < 0.2)=μ(z = 0.2)= − 1.29 ± 0.09 (details in text).
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