Fig. 7
The galaxy stellar mass function at z = 0 split by environment, defined by host halo mass (top) or group richness (number of companions with mstars > 1010 M⊙/h in the same host halo, bottom). The dashed curves in the top panel show the conditional mass function fits to the SDSS data by Yang et al. (2009). The same h and IMF corrections as in Fig. 6 apply.
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