Fig. 15
Number of sub-halos as a function of the projected distance from the cluster lens centre (right) and as a function of circular velocity (left) within an aperture of ~ 400 kpc for our best-fit model of MACS J0416.1–2403 (grey filled) as compared to the model of Grillo et al. (2015) (red) and to the median values and the 1σ uncertainties obtained from cosmological simulations used therein (Bonafede et al. 2011; Contini et al. 2012; Grillo et al. 2015).
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