Projected galaxy number density profiles n(R) (symbols with 1σ error bars) and best-fits (solid lines) for the whole cluster population (black filled dots), for the population of passive cluster galaxies (red open dots), and for the population of SF cluster galaxies (blue stars). The best-fit models are pNFW for all and passive members, and the model of King (1962) for the SF members. A constant galaxy density background is added to all models. The vertical magenta dashed line represents r_200,U.