Fig. 3.
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Cumulative galaxy mass function for the HR_HYDRO, HR_DMONLY, LR_HYDRO, and LR_DMONLY simulations at redshift 0 for the four bins in mass considered. The shaded regions correspond to the standard deviation across clusters. Resolution effects are clearly visible for the low-mass region. The vertical lines represent the minimum relative mass necessary to avoid resolution effects. (a) MB1, (b) MB2, (c) MB3,(d) MB4.
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