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Fig. 10.

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Total IR (8−1000 μm) luminosity or SFR as a function of redshift for the PHz-IRAM sources (full red stars for secure line identifications and full blue stars for uncertain line identifications) and for 1.4 < z < 3.1 cluster and protocluster members from the literature (gray triangles and crosses). In the case of multiple EMIR detections associated with the same SPIRE source, an upper limit to LIR was reported with a downward pointing arrow. Blue stars connected with a solid blue line refer to the same source and to two possible redshifts. The black dashed line represents the total IR luminosity of a source with S(350 μm) = 40 mJy and Tdust = 30 K (derived using the cmcirsed package; Casey 2012) corresponding to the selection of the majority of the PHz-IRAM targets. The dotted line is the same LIR limit scaled by −0.2 dex and used to select a subset of cluster and protocluster members from the literature for comparison (gray triangles).

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