Fig. B.2.

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Time evolution of Mg vs Mstar over the last 50% of the galaxies’ lifetime, according to the toy-model based on three exponential SFHs: β = ( − 1, 0, 1), and also assuming that the SFR timescale τSF is the same as the gas depletion time, τg = . Galaxy age tgal is given by Eq. (B.4), ψ0 by Eq. (B.3), and the Mg evolution by Eq. (14). The median curves in different Mstar bins are plotted, where the (median observed) gas mass Mg is taken to be Mg(tgal). For Δη = α, the equilibrium solution, Mg = Mi throughout the lifetime of the galaxy.
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