Fig. 10.
Average number of satellite galaxies, with Ms in range of [10−3, 1] of Mc, as function of halo mass. Here, Ms and Mc are the masses of satellites and centrals. Four lines denote the results at four redshifts derived from the conditional stellar mass function (CSMF) shown in Moster et al. (2010). The triangles and stars represent the results derived from the CSMFs of Reddick et al. (2013) and Yang et al. (2009), respectively.
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