Fig. 14
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Identification of cluster membership with S-PLUS photometric redshifts. The top row contains the sky projection of the S-PLUS data galaxies (PROB_GAL ≥ 0.5) obtained from a cone-search centred in the cluster coordinates. The middle row contains the photometric redshift distribution for these clusters, and the bottom row shows the objects selected based on a cut on photometric redshifts.
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