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Table 3.
Parameters describing the stellar mass–size relation of quiescent galaxies and its evolution since z ∼ 1, see also Eq. (4), and their uncertainties for BC03 and EMILES (including BaSTI and Padova00 isochrones) SSP models.
| β | γ | δ | |
|---|---|---|---|
| Padova00 | 0.71 ± 0.02 | −0.41 ± 0.02 | 0.60 ± 0.01 |
| BaSTI | 0.75 ± 0.02 | −0.42 ± 0.02 | 0.57 ± 0.01 |
| BC03 | 0.68 ± 0.02 | −0.46 ± 0.02 | 0.75 ± 0.01 |
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