Fig. 14
Star formation rates versus stellar masses and B-magnitude in intervals of 1 Gyr in comparison to the dwarf galaxies from Weisz et al. (2012), Huang et al. (2012) and McQuinn et al. (2015) for the left panels, and in addition for the right panel from Ott et al. (2012), Warren et al. (2012), and Hunter & Elmegreen (2006). Note that the stellar mass grows during the simulations.
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