Same as figure 6, top and middle panels, but for the different simulations. Shown are the cumulative relative cluster density as a function of distance from the MW position obtained from the simulations: SLOW (solid), CORUSCANT (dashed), SIBELIUS (long dashed), and early CLUES (dash-dotted). The blue lines are for very massive halos and the red lines are for clusters and correspond to the observations from the CLASSIX Böhringer et al. (2020) sample.