Fig. 2.

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Projected phase-space diagram of the galaxies in the field of PSZ2 G044.20+48.66 (Abell 2142) and member selection. The distance Dc is the angular diamater distance to the cluster. This is the CHEX-MATE cluster with the greatest number of confirmed redshifts in the virialised region. The initial candidates within a radial distance of 3θMMF3, 500c from the X-ray peak, and within a window in velocity of ±Δvrf, PSZ2 with Δvrf, PSZ2 = 12 000 km s−1 from the nominal PSZ2 estimate, are shown in orange. The virialised members (in blue) are selected within a radial distance of r200c and a rest-frame velocity window of ±κσlos(R), with κ = 2.7, where σlos is the velocity dispersion along the line-of-sight at projected radius R. Radial distances are shown assuming the final cluster redshift.
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