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Fig. 16


Total star formation rate (SFR) per Planck IN region, i.e., for the overdensity sample, assuming each overdensity is an actual high-z cluster of dusty galaxies, located at a redshift given by the SPIRE photometric redshift, and using a modified blackbody fit with a fixed dust temperature of Td = 35 K (purple, right histogram peaking at 7 × 103M yr-1), this temperature being favoured by the literature. We also show the total SFR for Td = 25 K, giving a peak at 2 × 103M yr-1. The structures could be intensively star-forming clusters. See Sects. 6.3 and 6.4 for details.

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