The fraction of each profile type (I, II, III) according to the angular projection within the cluster (from red to yellow) similar to Fig. 11 but for three different stellar mass bins from left/lower masses to right/larger masses as labelled. Error bars represent the 1σ binomial uncertainties calculated as $\sigma =\sqrt{f(1-f)/N}$, where f is the measured fraction and N is the total number of galaxies in the corresponding bin.