Fig. 4
BCG stellar mass versus total halo mass. Black dots show lines of constant stellar mass fractions of 0.0001, 0.001 and 0.01. -signs show the results from Hilton et al. (2013). The relation is the best fit to the combined data set of Hilton et al. (2013) and the current study. Estimates from Behroozi et al. (2010) and Behroozi et al. (2013) are indicated by the shaded regions.
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