CHEX-MATE: Exploring the kinematical properties of Planck galaxy clusters

Open Access

Fig. 1.

Cluster redshift and $M_{500}^{SZ}$ $M_{500}^{\mathrm{SZ}}$ mass distributions of the full CHEX-MATE sample (red) and the subsample (blue). $M_{500}^{SZ}$ $M_{500}^{\mathrm{SZ}}$ has been derived iteratively from the $Y_{SZ} - M_{500}^{SZ}$ $Y_{\mathrm{SZ}}{-}M^{\mathrm{SZ}}_{500}$ relation calibrated using hydrostatic masses obtained from XMM-Newton data (see CHEX-MATE Collaboration 2021).

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