0.3−30 keV luminosity at the end of the energy-injection phase (Dainotti et al. 2008). The black dots are taken from Margutti et al. (2013). The stars correspond to the GRB 121024A afterglow: the red star to when the end of the plateau phase lies at 49.8 ks, the green star corresponds to the ongoing energy-injection phase before and after the break in the LC at t = 240 ks, and the grey star corresponds to the luminosity corrected for the jet-break effect. The dashed line in the middle corresponds to the best fit, and the shaded region is the 1σ error of the fit.