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Fig. 4.

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Comparisons between the CHIMF of satellite galaxies from the different simulations. The labels are the same as in Figure 1. Results from Li et al. (2022) are plotted in solid purple lines. Within the mass interval 12 < log(Mvir/M) < 14, the halo count in GAEA is similar to that in SIMBA, whereas TNG has only about 50% as many as SIMBA.

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