Fig. 4.
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Comparison of M500c − M* relations of central star-forming (top) and quiescent (bottom) galaxies in the catalogs of Tinker (2021) and Yang et al. (2007), and EAGLE, TNG100, and SIMBA simulations. The shadow area denotes the 16–84% scatter of the relation. Yang et al. (2007) only includes galaxy groups with log(M500c) > 11.5 and causes the turnover of the quiescent SHMR at low mass end.
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