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Fig. 4.
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Ratio of post-to-pre re-ionisation stellar mass (M★, post/M★, pre) as a function of total stellar mass for galaxies in NIHAO (top) and FIRE-2 (bottom) simulation suites. Dashed black lines show second-degree polynomial fits. Circles are coloured by their relative deviation from the fit, which we define as SFH deviation.
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