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Fig. 7.

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Galaxy stellar mass function for the star-forming (top panel) and quiescent galaxies (bottom panel) in clusters at 1 < z < 1.4. Solid lines show predictions from the models considered in this study, as indicated in the legend. Symbols with error bars show corresponding observational estimates published in van der Burg et al. (2020). The shaded regions show the area enclosed by the 10th and 90th percentiles of the distributions of number densities obtained, for each galaxy stellar mass bin, when considering 25 samples of simulated haloes that match the mass and redshift distributions of the GOGREEN sample (see text for details). All model lines shown in this figure assume an uncertainty in stellar mass of 0.25 dex.

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