Fig. 13.
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Constraints on cosmological parameters (H0, Ωm, σ8) from the Planck PSZ2 cluster number counts and BAO data, with three different completeness functions: the “standard” ERF completeness (same as in Planck Collaboration XXIV 2016), and two “fitted” versions obtained by rescaling the noise per patch by a constant in order to reproduce the completeness derived from the simulation clusters and the PACT (Pointecouteau et al. 2021) profile clusters. The filled contours represent 68% and 95% confidence regions.
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