Left: B-band TFR. Colored stars represent the different cluster samples that compose our study. The solid black line shows the local B-band TFR (Tully et al. 1998) with a 3σ scatter area reported by Böhm & Ziegler (2016) for galaxies at 0 <  z <  1 (gray area). Right: B-band TFR offset evolution. Stars with colored edges represent the distribution of our cluster samples, and their respective mean values are shown as larger circles of the same color. Error bars represent the error of the mean for every sample. Open circles display the Böhm & Ziegler (2016) field sample at 0.1 <  z <  1. We binned the field sample into three redshift intervals (0 <  z <  0.33, 0.33 <  z <  0.66, and 0.66 <  z <  1). Black circles depict the mean value and its error for the field sample in every redshift window. The dashed line represents the predicted B-band luminosity evolution by Dutton et al. (2011) in the TFR, and the dash-dotted line at ΔM_B = 0 means no size evolution.