Projected number density of all members of the comparison clusters and A 520. These are completeness corrected kde densities estimated separately for passive, active and recently quenched galaxies using the same smoothing kernel size. log (ρ_proj) of the passive galaxies is shown as an underlying image, of the star forming galaxies with solid contours, and of the recently quenched ones with dashed contours. The contours are drawn at the levels indicated with the tick marks on the colour bar. The green circle has a radius equal to R₂₀₀ of the given cluster.