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Table A.1.

Parameters μ(z, M) and σint(z, M) of probability distribution functions of luminosity and mass-weighted ages in real space (Gyr units, see Eq. (A.2)).

AgeL [Gyr] Ngal μAgeL

μ1 μ0 σ1 σ0
10.0 ≤ log10M <  10.4 1429
BC03 10.4 ≤ log10M <  10.8 2526
10.8 ≤ log10M <  11.2 3181
log10M ≥ 11.2 1122

10.1 ≤ log10M <  10.5 1284
EMILES+BaSTI 10.5 ≤ log10M <  10.9 2370
10.9 ≤ log10M <  11.3 3089
log10M ≥ 11.3 1159

10.1 ≤ log10M <  10.5 1329
EMILES+Padova00 10.5 ≤ log10M <  10.9 2335
10.9 ≤ log10M <  11.3 2945
log10M ≥ 11.3 1141

AgeM [Gyr] Ngal μAgeM

μ1 μ0 σ1 σ0

10.0 ≤ log10M <  10.4 1429
BC03 10.4 ≤ log10M <  10.8 2526
10.8 ≤ log10M <  11.2 3181
log10M ≥ 11.2 1122

10.1 ≤ log10M <  10.5 1284
EMILES+BaSTI 10.5 ≤ log10M <  10.9 2370
10.9 ≤ log10M <  11.3 3089
log10M ≥ 11.3 1159

10.1 ≤ log10M <  10.5 1329
EMILES+Padova00 10.5 ≤ log10M <  10.9 2335
10.9 ≤ log10M <  11.3 2945
log10M ≥ 11.3 1141

Notes. These were derived using BC03, EMILES+BaSTI, and EMILES+Padova00 SSP models. The top and bottom numbers establish the 1σ confidence level of the parameters.

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