Fig. 2.
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RAR for selected Milky Way (blue) and Andromeda (orange) satellite dSphs and galaxy clusters (green). Uncertainties are 1σ. The data are taken from Lelli et al. (2017) for the dSphs (Milky Way and Andromeda satellites) and Li et al. (2023) for the galaxy clusters, as is tabulated in Tables A.1 and B.1, respectively. The bold grey lines for different p are the same as in Fig. 1.
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