Fig. 7.
Stellar-to-halo-mass relation (top) and halo mass-concentration relation (bottom). The black solid line and the gray shaded areas show the relations expected in ΛCDM together with their intrinsic scatter (Moster et al. 2013; Dutton & Macciò 2014). The solid points with ±1 sigma errorbars show the maximum-probability values from rotation-curve fits with ΛCDM priors.
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