Table 2.
Slope α = −b/a of constant stellar population properties of quiescent galaxies in the stellar mass–size plane, see Eq. (3).
EMILES | EMILES | BC03 | |
---|---|---|---|
(Padova00) | (BaSTI) | ||
AgeM + tLB | 0.55 ± 0.10 | 0.50 ± 0.07 | 0.54 ± 0.09 |
AgeM | 0.55 ± 0.07 | 0.50 ± 0.09 | 0.55 ± 0.07 |
[M/H]M | 0.43 ± 0.13 | 0.33 ± 0.26 | 0.34 ± 0.25 |
Notes. Stellar population parameters were obtained for the SSP model sets of Bruzual & Charlot (2003, BC03) and Vazdekis et al. (2016, EMILES), the latter including BaSTI and Padova00 isochrones. From top to bottom, mass-weighted formation epoch, age, and metallicity.
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