Fig. 7.
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MEHs and SFHs of all galaxies with log10(M*/M⊙) < 11 together, divided according to their SFH, between galaxies that formed within Δτ = τ95 − τ5 = lower and greater than 1 Gyr. Since we are considering galaxies at all redshifts, given the mass completeness limit, the statistics are biased toward higher-mass galaxies. The hatched region indicates the 16th percentile of galaxies in the lowest mass bin, 10.4 ≤ log10(M*/M⊙) < 10.6.
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