Fig. B.2.
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Same as Fig. 11, but for the Magneticum galaxy clusters using three different definitions of the split between ICL and BCG. Left panel: Same as the left panel of Fig. 11, but with a split between BCG and ICL at 0.1 ⋅ R200, cri. Central panel: BCG and ICL split at 3 ⋅ R*, 1/2, with R*, 1/2 the stellar half mass radius. Right panel: BCG and ICL split at a fixed aperture of 100kpc.
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