Fig. 4.
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Ratio of the fluxes contributed by the ICL and BCG components of the model clusters measured within both the 50–200 kpc annulus (red points) and a 100–200 kpc annulus (blue points) as a function of halo mass. Each point shows, for a given cluster, the total ICL flux within the annulus divided by the total BCG flux within the annulus.
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