Correlation diagram between the offsets, ΔM_B, from the TFR and the offsets, Δlog R_d, from the VSR for previously presented samples. The solid line shows the linear fit for galaxies studied in the local Universe (Haynes et al. 1999b). By definition, this line goes through the coordinates origin. The dashed black lines plotted in this diagram show the linear fit for galaxies studied in Böhm & Ziegler (2016) at 0.59 <z< 1, showing that galaxies are shifting away with lookback time toward higher luminosity and smaller sizes. The dotted black line is the linear fit at a fixed slope for our cluster sample, whose zero-point is shifted by –0.69 dex in Δlog R_d with respect to the local sample.