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Are short y-ray bursts collimated GRB 050709, a flare but no break
(2006)
Context. From the small sample of afterglow lightcurves of short duration γ-ray bursts (GRBs), the decays are rapid, roughly following a power-law in time. It has been assumed that the afterglow emission in short GRBs is ...
GRB 050814 at z = 5.3 and the Redshift Distribution of Swift GRBs
(American Institute of Physics (AIP), 2006)