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 different galaxy morphology from Hubble type −1 on the left-hand panel, to one on the right-hand panel. 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.