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Fig. A.2.

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Porcentual distributions stellar masses considering the baryonic masses. Stellar galaxy mass in rop aperture (upper row panels), ICL mass in rop aperture (upper centre row panels), stellar galaxy mass in Subfind aperture (bottom centre row panels) and ICL mass in Subfind aperture (bottom row panels). The histograms are divided in the haloes with log 10 ( M 500 c / M ) < 14 $ \log _{10}{\left ( M_{\mathrm {500c}} / {\mathrm {M_{\odot }}} \right )} < 14 $ (left colum panels), log 10 ( M 500 c / M ) 14 $ \log _{10}{\left (M_{\mathrm {500c}} / {\mathrm {M_{\odot }}} \right )} \geq 14 $ (centre colum panels) and all halo (right colum panels) masses. (Black histograms) TNG100 haloes. (Red histograms) TNG300 haloes. The dashed lines represent the normal distribution fitted in their respective histogram (with their respective colour).

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