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.
E., Springel, V ., White, S
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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.