Fig. B.2.
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Fraction of star-forming (blue) and quiescent (orange) galaxy samples as a function of mass at for three redshift ranges compared to simulations. We include measurements from UNIVERSE MACHINE Behroozi et al. (2019, sSFR < 10−11 ℳ⊙ yr−1) shown by dotted lines, as well as those from consistently NUVrJ-selected samples from EAGLE (Furlong et al. 2015) and SHARK (Lagos et al. 2018).
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