Notes. N_c is the number of clusters in the sample. N_M and N_m are respectively the sum of the membership weights and the total number of members with M_⋆ ≥ 10^9.5 M_⊙ in the clusters that are part of the sample, at all radii (Col. 3) and in the radial range used for the dynamical analysis (Col. 5). f_SF is the fraction of star-forming galaxies among the members in the 0.05 ≤ R ≤ r₂₀₀ radial range, identified based on their U − V and V − J rest-frame colors (for more details see text and van der Burg et al. 2020). z and r₂₀₀ are evaluated using N_M-weighted averages of the corresponding quantities for the clusters that are part of the sample. M₂₀₀ is derived from r₂₀₀, given z (see footnote 1).