Fig. 8

Comparison of the integrated properties of halos in our sample, as a function of halo mass, with model predictions from Béthermin et al. (2013, black), Leauthaud et al. (2012, green), and Behroozi et al. (2013, red): stellar mass fraction of satellites with respect to the central (top), stellar to total mass ratio (middle), and SFR fraction of satellites compared to that of the central (bottom; the dashed line corresponds to a case without environmental effects). The black circle and gray diamond show, respectively, the MF-corrected and uncorrected values. The latter have been shifted to the left for clarity.
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