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.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.