Fig. 2.
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Photometric cluster membership. Top: photometric redshift distribution of the galaxies in the region of SPT0615. Bottom: color-magnitude diagram with the members of SPT0615 at z = 0.97 in red and those of the possible foreground structure at z ∼ 0.44 in black. Gray points correspond to interlopers that do not belong to any of the two structures.
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