Fig. 13.
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Lower panels: cGSMFs of the group galaxy subsample colour-coded by Mdyn as indicated in the legend. In panel (a), we use the MassA calibration factor, while in panel (b) we use the MassAfunc factor. For comparison, the cGSMF of the ungrouped galaxies is also shown in brown. Upper panels: Raw number of galaxies as a function of stellar mass in each sample, as indicated.
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