Fig. 3.

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Projected stellar mass density maps of two DIANOGA PC regions, which are the progenitors of clusters of total mass M200c equal to 5 × 1014 M⊙ and 2 × 1015 M⊙ at z = 0 (left and right panel, respectively). In each panel, the larger red dashed circle corresponds to the PC region as defined in the text, while the smaller circles show the R200c of halos in these regions with M200c > 1013 M⊙. Densities are computed in pixels of size 15 (10) kpc in the right (left) panel.
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