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Fig. 9


Characteristic halo masses from the best-fitting HOD models of the correlation function selected in luminosity vs. LthreshL* (left panel) and selected in stellar mass vs. MthreshM* (right panel). Minimum halo masses Mmin for which 50% of haloes host one central galaxy above the threshold limit (filled symbols) and masses of haloes which on average host one additional satellite galaxy M1 (open symbols) observed at z ~ 3 are compared with similar results found by Zehavi et al. (2011) at z ~ 0, for the luminosity selected galaxies, and by Skibba et al. (2015) at z ~ 0.5, for the stellar mass selected galaxies (dotted and dashed lines).

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