Fig. 13.

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Mean halo occupancy of BGS (top-left panel), LRG (top-right panel), ELG (bottom-left panel), and QSO (bottom-right panel) samples, as determined from our (modified) SHAM UCHUU lightcones. The mean number of galaxies of a halo with a given mass Mhalo is denoted by 〈Ngal〉. The solid lines represent the combined centrals and satellite occupation, while the dotted and dashed lines show the mean halo occupancy for centrals and satellites, respectively. The shaded area indicates the 1σ uncertainty of the occupation measured from the UCHUU lightcones. For BGS, this is a jackknife error from the full-sky mock, split into 100 jackknife regions. For the other tracers, this is the 1σ scatter between the 102 mocks. The best-fit HOD model parameters for BGS and LRG are listed in Tables 4 and 5, respectively.
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