CS-SHAM with three free parameters for satellite fraction reproduces galaxy clustering across different subhalo proxies and shows that clustering mainly constrains the halo occupation distribution for massive halos.
For satellite galaxies, both models successfully reproduce the ELUCID SAM CSMF in halos with logM h ≳12.9
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What can galaxy clustering really tell us about the galaxy-halo connections?
CS-SHAM with three free parameters for satellite fraction reproduces galaxy clustering across different subhalo proxies and shows that clustering mainly constrains the halo occupation distribution for massive halos.