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Broad-Band Modelling of GRB Afterglows

Berger, Edo and Sari, Re’em and Frail, Dale and Kulkarni, Shri (2001) Broad-Band Modelling of GRB Afterglows. In: Gamma-Ray Bursts in the Afterglow Era. ESO Astrophysics Symposia. Springer , Berlin, pp. 154-156. ISBN 978-3-540-42771-1. https://resolver.caltech.edu/CaltechAUTHORS:20191008-153238185

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Abstract

Observations of GRB afterglows ranging from radio to X-ray frequencies generate large data sets. Careful analysis of these broad-band data can give us insight into the nature of the GRB progenitor population by yielding such information like the totalenergy of the burst, the geometry of the fireballand the type of environment into which the GRB explodes. We illustrate, by example, how global, self-consistent fits are a robust approach for characterizing the afterglow emission. This approach allows a relatively simple comparison of different models and a way to determine the strengths and weaknesses of these models, since all are treated self-consistently. Here we quantify the main di?erences between the broad-band, self-consistent approach and the traditional approach, using GRB000301C and GRB970508 as test cases.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/10853853_40DOIArticle
ORCID:
AuthorORCID
Berger, Edo0000-0002-9392-9681
Kulkarni, Shri0000-0001-5390-8563
Additional Information:© 2001 Springer-Verlag Berlin Heidelberg. First Online 14 October 2003.
Series Name:ESO Astrophysics Symposia
Record Number:CaltechAUTHORS:20191008-153238185
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20191008-153238185
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:99167
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:08 Oct 2019 22:45
Last Modified:08 Oct 2019 22:45

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