Fig. 1.

Top panel: redshift distribution of our PSZ2 sample (1091 clusters). Bottom panel: predicted cluster dust flux density versus redshift from the De Zotti et al. (2018) model. The dust emission is integrated within a sphere of radius R500 for a cluster of mass M500 = 1014.5 M⊙ in the 857 GHz Planck band. We fixed rL = 1 (see Eq. (5)) in this figure.
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