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.
It produces quasi-uniform samples in high-dimensional spaces via binary radical inversion, making it particularly well suited for MCMC applications
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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.