Fig. 1.
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X-ray light curves of SGRBs with viewing angle 0 ° < θv < 15° predicted by our model. The lines are produced with a random extraction from the posterior distribution of prompt parameters. In the computation we assume Stru1 and we include both HLE and FS (configuration FS-SGRB). The color of each line indicates the viewing angle. The X-ray luminosity is computed at 5 keV.
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