Fig. 8
Contribution of each halo mass range to the CSFH as a function of redshift. The CSFH of the Universe is taken from Magnelli et al. (2013). The shading indicates the 1σ confidence level as derived in Magnelli et al. (2013). The shaded green, magenta, and black regions show the contributions of the low mass group, high mass group, and cluster galaxy populations, respectively. The black points show the compilation of Hopkins & Beacom (2006).
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