Fig. 25
Same as Fig. 9, but for RXC J2308: substructure candidates (regions G*), regions used to estimate the density of field galaxies (R1 and R2), and contours tracing the surface density of the bright red-sequence galaxies. Symbols show the location of the spectroscopic members associated with the different KMM partitions. The dashed circle has a radius of R200 ~ 2.3 Mpc.
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