Fig. 7.
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Inferred stellar-to-halo-mass relation for each sample observed. The stars are located at the median values. The distributions of the halo and stellar masses of the sample studied are shown with colored solid lines. There is a fair agreement with previous models Yang et al. (2005), Tinker (2021) and with the prediction from the TNG and SIMBA hydrodynamical simulations (Pillepich et al. 2018; Davé et al. 2019; Schaye et al. 2015).
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