Fig. 3
g′-r′ versus r′ for the CFHTLS objects in a 5′ square (allowing a ~1 Mpc radius at the cluster redshift) around the XLSSC 116 cluster centre. Points are all the detected objects; filled circles are the galaxies with a MUSE measured spectroscopic redshift (red: SG substructure 1, blue: SG substructure 2, see Sect. 4.2). The large blue octagon is the sum of all the diffuse light components in the cluster.
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