Fig. 15

Left panels: halo mass estimates Mmin and M1 for all (top) and red (bottom) galaxy samples, as function of luminosity threshold, corrected for passive redshift evolution to approximate stellar mass selected samples. The dashed lines correspond to Eq. (25). Right panels: light-to-halo mass ratios (Eq. (26) with identical parameters as those fitted with Eq. (25)) as function of halo mass.
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