Fig. 5
Stellar mass density distribution of the ensemble cluster at z ~ 0.15. Black points: cluster stellar mass distribution, with best-fitting projected NFW (dashed) and gNFW (solid) functions. Purple points: stellar mass distribution in spectroscopically confirmed cluster members. Dotted line: total stellar mass density profile on the images (background subtracted, with the 68% confidence region around these values shown by the thinner dotted lines), including the BCG and part of the ICL component.
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