Fig. 6


Non-parametric halo occupation distribution of satellite galaxies in XXL-100-GC clusters in three temperature bins as a function of the galaxy’s stellar mass for three temperature bins (T300 kpc< 3.5 keV, blue; 3.5 <T300 kpc< 4.8 keV, green; T300 kpc> 4.8 keV, red).

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