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Table 3.

Fit to the median age and metallicity as a function of stellar mass for the general population.

Parameter Sample P ¯ Mathematical equation: $ \bar{P} $ A B M * ¯ [ M ] Mathematical equation: $ \bar{M_\ast}\,[M_\odot] $
log⟨Age/yr⟩r LEGA-C silver 9.62 ± 0.04 0.3 ± 0.1 2 ± 1 1.2 ± 0.4 ⋅ 1011
LEGA-C golden 9.66 ± 0.02 0.30 ± 0.02 2.4 ± 0.3 1.07 ± 0.09 ⋅ 1011

SDSS-SN10 9.782 ± 0.002 0.289 ± 0.005 1.28 ± 0.04 6.5 ± 0.2 ⋅ 1010

log⟨Z*/Zr LEGA-C silver 0.37 ± 0.04 0.8 ± 1.4 1.6 ± 1.3 1 ± 2 ⋅ 1010
LEGA-C golden 0.46 ± 0.01 1.0 ± 1.7 1.2 ± 0.6 0.9 ± 2 ⋅ 1010

SDSS-SN20 0.435 ± 0.004 0.46 ± 0.08 0.8 ± 0.1 1.0 ± 0.4 ⋅ 1010

Notes. Relations fit to the median age and metallicity as a function of stellar mass using the functional form of Eq. (3) for the silver and golden LEGA-C samples as well as for SDSS DR7 (with S/N > 10 and S/N > 20 for age and metallicity, respectively) displayed in the left panels of Figs. 5 and 7. The columns list (1) the parameter, (2) the sample, (3) the characteristic parameter P ¯ Mathematical equation: $ \bar{P} $ at 1011.5M, (4) the A parameter that regulate the age/metallicity increase over the inflection, (5) the B parameter that regulates the mass range of inflection, and (6) the characteristic mass M * ¯ Mathematical equation: $ \bar{M_\ast} $ of the inflection point.

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