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Fig. 5.

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Cumulative distribution of the mass contribution to the post-stripped ICL from halos of different infall masses. The left column is for stellar mass at infall; the right column is for the total mass ratio to the host at infall time. The lines depict the distributions obtained as the median of the individual distributions for each cluster, while the shaded regions indicate the 16th–84th percentiles. The green solid lines are for GADGET-X and the magenta dash-dotted lines for GIZMO-SIMBA. In the right column, the yellow and brown shaded regions indicate the minor (1:10 to 1:3) and major merger regimes (1:3 to 1:1). The horizontal dotted lines indicate fractions of 0.25, 0.5, and 0.75 of the post-stripped ICL.

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