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Fig. 4

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Histogram of the redshifts obtained for the initial candidate sample (black) and for the final sample of 292 robust cluster candidates, 21 spectroscopic and 271 photometric (red). The filled histogram represents the FIR-emitter sample. The dot-dashed line at 0.886 indicates the locus of the photometric redshift of the cluster, and the solid lines shows the final photometric range we have considered.

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