Left panel: TFR for our S0-like remnants in the B band at z ~ 0.8 using V_rot,max, compared to data of real spirals and S0 galaxies at high redshift. We include the error bars in the kinematics of the early-type galaxies by Jaffé et al. (2014) to highlight the uncertainties of the data at z ~ 0.8. Right panel: local TFR for our S0-like remnants at z ~ 0 using V_rot,max, in comparison with present-day S0 galaxies (see the legend below the figure). This figure is analogous to Fig. 5, but using the maximum rotational velocity measurements instead (see the caption there).