Fig. 7.
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Top: HMR for the three different components that make up the BCG+ICL, the component accreted from surviving galaxies, accreted in completed mergers and formed in situ. Bottom: HMR for the three different components that make up the ICL. Dashed lines on the histograms indicate the median. The slopes of the linear fit to the data, β, are indicated in the lower middle panel.
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