PPS of major cluster-member populations of this work, re-scaled by the mean value of R_200c and v₂₀₀. The scale at the right of every plot represents the number of objects in each bin. We note that the blue galaxies, as expected, are more concentrated towards the outer regions of our ensemble cluster, while the red ones are mostly found in the inner regions. The HM population, despite it being radially distributed almost the same as the LM population, is slightly less spread out in terms of velocity than the latter.