Fig. 4
Rest-frame, (0.3−10) keV, and re-binned luminosity light curves of GRB 130427A (upper left), GRB 061121 (upper right), GRB 060729 (lower left) and a combined picture (lower right). The fits to their emission is done using a power-law function for the early steep decay and a phenomenological function for the following emission, which is described well in Ruffini et al. (2014a).
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