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Physical Constraints From Broadband Afterglow Fits:GRB000926 as an Example

Sarah A. Yost·Re'em Sari·Fiona A. Harrison·Edo Berger·Alan Diercks·Titus Galama·Dan Reichart·Dale Frail·Paul A. Price
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Abstract

We develop a model to fit the broadband afterglows of GRBs from the intrinsic parameters of the fireball's synchrotron emission, and apply it to a few well-studied events, with the goal of constraining the intrinsic variability of GRB parameters. We give an example here of fitting to the recent bright event GRB000926.

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Sarah A. Yost, Re'em Sari, Fiona A. Harrison, Edo Berger, Alan Diercks, Titus Galama, Dan Reichart, Dale Frail, Paul A. Price. 2001-07-29. Physical Constraints From Broadband Afterglow Fits:GRB000926 as an Example. https://doi.org/10.1007/10853853_56

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