Fig. 8.
Marginalised posterior distributions for AT − M and (1 − b) calibration parameters, for combination of CMB, SZ and X-ray cluster data in various cosmological models: with or without massive neutrinos, with or without free growth index γ, and free σ8. For the ΛCDM and νγCDM models, the dashed lines show the same posterior obtained when using the Planck 2018 CMB data instead of the 2015 one.
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