Fig. 1

Distribution of the galaxies of Abell 2142 in the projected phase-space of projected radii and LOS rest-frame velocities. Cluster members, as identified by both dHK and clean algorithms, are denoted by blue filled dots. The red diamond is the galaxy identified as member by dHK but not by the clean algorithm. The purple solid lines are the caustic, described in Sect. 3. The vertical dashed line locates the virial radius of the combined model (see Sect. 4).
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