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Fig. B.1.

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Galaxy stellar mass functions for total (gray), star-forming (blue), and quiescent (orange) samples from this work compared to simulations. We include those from UNIVERSE MACHINE Behroozi et al. (2019, sSFR < 10−11 ℳ yr−1) shown by dotted lines with hatched uncertainty envelopes, as well as consistently NUVrJ-selected samples from EAGLE (Furlong et al. 2015) and SHARK (Lagos et al. 2018) shown by the dashed and dot-dashed lines, respectively. Upper limits for empty bins are shown by the horizontal gray line with an arrow. Mass incomplete measurements are not shown.

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