Fig. C.1.
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Star formation history (top) and star formation rate history (bottom) derived for NGC 1365 (left) and NGC 1566 (right). The best-fitting linear model for the SFH curve of each galaxy is shown as a red dashed line, and its slope and intercept are shown in the top-left corner of the top panels. The shaded areas mark sudden decreases in the SFR at ages log (age/yr) ∼7.7 and log (age/yr) ∼9.5, found to exist in all galaxies in some degree, deemed as an artifact of the computed SFHs.
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