Example illustration of the modeling of the SFR density profiles described in Sect. 5.4, see text for full details. Left, middle and right panel: three different values assumed for the r <  r₅₀₀ quiescent fraction above mass completeness, as indicated. Top panels: radial profile of quiescent fraction above mass completeness (black, the field value is shown in gray). The dotted red line shows the quiescent fraction of the full mass complete sample out to the given clustercentric radius. Middle panels: projected galaxy number density profile above mass completeness (black), and the derived profiles of star-forming and quiescent galaxies (blue and red) given the quiescent fraction profile in the corresponding top panel. Bottom panels: corresponding projected SFR density profiles, derived with the two models of quiescent fraction vs. stellar mass as indicated (solid lines). Dashed and dotted lines show the additional SFR density profile over the prediction for the actually observed quiescent fraction (see text). Inserts show the corresponding cumulative SFR as a function of clustercentric radius.