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Fig. 8.

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Galaxy distribution as a function of the host halo mass. Top: Total (central + satellite) number of galaxies contained in halos as a function of halo mass, M, evaluated at the sample median redshift. The four curves correspond to the different stellar mass threshold bins. The shaded bands represent the 1σ uncertainty. Middle: Total number of galaxies per comoving volume and halo mass range (in units of Mpc−3 ) as a function of halo mass. Bottom: Total number of galaxies per halo mass range normalized by the number of galaxies in each stellar mass bin. This fraction of galaxies lies in a halo of mass M. The quantity V appearing in the label stands for the comoving volume.

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