Left panel: TFR for our S0-like remnants in the B band at z ~ 0.8, using V_circ. Right panel: TFR for our S0-like remnants at z ~ 0 after ~7 Gyr of passive evolution of their stellar populations (accounting for the effects of the residual star formation in the remnant since z ~ 0.8) compared to present-day spiral and S0 galaxies, also using V_circ. We have distinguished between the remnants of prograde and retrograde encounters. Data are labelled as shown in the figure. In both panels, the dotted line denotes the local TFR in the B band for spiral galaxies by Williams et al. (2010a), whereas the dashed line corresponds to the local TFR in the B band for S0 galaxies also by Williams et al., and the yellow band its 1σ scatter. The error bar in the bottom left corner of each panel denotes the statistical errors on both axes for our S0-like remnants.