Table 2.
Samples used in the scientific analysis and mean uncertainties on the physical parameter estimates.
| Sample | NQ | NSF | mean σlog⟨Age/yr⟩r [dex] | mean σlog⟨Z*/Z⊙⟩r [dex] | mean σlog(M*/M⊙) [dex] | mean σAg [mag] | ||||
|---|---|---|---|---|---|---|---|---|---|---|
| Q | SF | Q | SF | Q | SF | Q | SF | |||
| silver | 232 | 320 | 0.16 | 0.16 | 0.19 | 0.35 | 0.12 | 0.13 | 0.24 | 0.38 |
| golden | 148 | 175 | 0.15 | 0.15 | 0.15 | 0.29 | 0.11 | 0.12 | 0.21 | 0.36 |
Notes. (1) Samples (silver: all LEGA-C with primary = 1, flag_spec = 0, sigma_star > 0, 0.55 < z_spec < 1.1, and at least one of (Hβ, HδA, HγA) and one of ([Mg2Fe], [MgFe50]′, [MgFe52]′, [MgFe]′); golden: all silver galaxies with S/N > 20); (2) and (3) number of unique galaxies classified as quiescent (Q) or as star-forming (SF) according to their specific SFR (i.e. lying below or above, respectively, of the dashed line in the left panel of Fig. 2); (4) mean error on light-weighted age (dex); (5) mean error on light-weighted stellar metallicity (dex); (6) mean error on stellar mass (dex); (7) mean error on dust attenuation (mag). The mean errors are given separately for Q and SF galaxies.
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