Projected phase-space diagram of the 427 galaxies selected as members of the M1206 cluster (other clusters are shown in Fig. A.1) by the CLUMPS method in the region R ≤ 1.36 r₂₀₀. The three numbers at the bottom left indicate, from left to right, the number of galaxies selected for the dynamical analysis (black-circled green dots); the number of CLUMPS members that are excluded from the dynamical analysis because they are at R ≤ 0.05 Mpc, which is the region dynamically dominated by the BCG (red circles), and the number of CLUMPS members that are not used in the dynamical analysis because they are flagged as interlopers by the escape-velocity criterion (gray circles). The vertical lines indicate R = 0.05 Mpc and R = r₂₀₀. The values of r₂₀₀ and v₂₀₀ come from U18.