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Fig. B.1.
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Inferred galaxy age tgal plotted against Mstar for MAGMA galaxies (top panel); initial SFR at t = 0, ψ0 plotted against Mstar (middle); τg (assumed equal to τSF) plotted against Mstar (bottom). In the two top panels, we assumed a simple declining exponential SFH with β = −1 [Eq. (B.1)], and that 
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