Fig. 7.
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Stellar-to-halo mass relation, as defined by Eq. (19), using the best-fit HOD parameters from our 2 × 2 pt+SMF analysis (blue). The result can be compared to results from Leauthaud et al. (2012, green), Moster et al. (2013, black), Coupon et al. (2015, orange), and van Uitert et al. (2016, purple). The grey area shows the range in stellar masses where the obtained stellar-to-halo mass relation is extrapolated beyond the range of median stellar masses used in this analysis.
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