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Fig. 5.

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Subhalo HOD shapes for various mass thresholds. Left: average number of subhalos in a parent halo as a function of parent halo mass for several peak virial (sub)halo mass limits. The solid colored lines correspond to the fitted powerlaw in the parent halo mass range 1013 < MVir < 5 × 1014h−1M. Right: HOD slopes (α) of each subsample of subhalos, showing the apparent decline of α with mass threshold.

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