Cumulative and differential distribution of de Vaucouleurs’t (left panel), of M_V (middle), and ratio aperture to effective radius log (d_fib/R_e), for cluster members (black) and non-cluster galaxies (gray). Top row of panels: all cluster and non-cluster galaxies included in the present study (i.e., w1 and w0 samples); second row of panels from top: cluster member vs. CS with matched distributions of M_V and de Vaucouleurs’ t (w0_t,M); third row from top: cluster member vs. CS with matched distributions of R_e and de Vaucouleurs’ t (w0_t,Re). Bottom row: resampled CS matching M_V, t, and R_e().