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Fig. 3


The zp distributions for the IR-emitting galaxies with available z in the supercluster field. The solid black (respectively, dashed blue) histogram represents the zp distribution for the galaxies selected as members (respectively, not selected as members) on the basis of their z. The two vertical red dash-dotted lines identify the lower and upper zp limits used to identify supercluster members in the sample of galaxies without z (not shown here).

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