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Fig. 7


From left to right: exponentially declining (a), exponentially rising (b), delayed (c), and log-normal (d) SFH considering a galaxy with a stellar mass of 6.3 × 1011M at z = 0. We compare the delayed and log-normal SFH shapes with our MS galaxy SFH in gray (see Fig. 5), in the last two panels. For the log-normal SFH, models are shown with lnt0 = 1 Gyr (solid lines) and lnt0 = 2 Gyr (dashed lines).

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