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Fig. 2


Observed triple correlations in 70 Swift GRBs with measured redshift, , , and Eiso and its best fit power law (straight line with a power law index − 0.58). Arrows indicate observational upper bounds on early time deceleration breaks before the beginning of the Swift/XRT observations or hidden under the prompt emission tail. The square represents the break in the late-time X-ray afterglow of GRB 980425 which was observed with Chandra.

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