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Fig. 8.

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CLF of all member galaxies (left panel), only central galaxies (central panel), and only satellites (right panel) as function of halo mass. The halo masses are split into five equally spaced logarithmic bins, whose median is reported in the legend. The samples of each group finder are marked with symbols whose legend is listed in the central panel, and the solid lines represent the input distribution from the SubFind halo catalogue.

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