Fig. 7.
Impact of dust emission on Planck cluster completeness as a function of redshift. The black line shows the completeness correction due to dust for the Planck MMF cosmological catalog (S/N > 6, Planck 65% cosmological mask; Planck Collaboration XXIV 2016) computed from Monte Carlo simulations. The error bands in red are obtained from 10 000 bootstrap realizations.
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