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GRB Prompt X-ray Emission

Published online by Cambridge University Press:  05 September 2012

Takanori Sakamoto
Takanori Sakamoto*
Affiliation:
Center for Research and Exploration in Space Science and Technology (CRESST), NASA Goddard Space Flight Center, Greenbelt, MD 20771, U.S.A. Joint Center for Astrophysics, University of Maryland, Baltimore County, 1000 Hilltop Circle, Baltimore, MD 21250, U.S.A. NASA Goddard Space Flight Center, Greenbelt, MD 20771, U.S.A. email: Taka.Sakamoto@nasa.gov
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Abstract

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I present the observational properties of the prompt emission of supernova associated GRBs (SN-GRBs) focusing on temporal and spectral characteristics. I compare the properties of SN-GRBs with typical long GRBs to see whether there is a distinct difference or not. Furthermore, I present our attempt to search for hard X-ray emission prior to the discovery date from optically identified type Ibc supernovae using Swift BAT survey data.

Keywords

gamma rays: bursts
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S279: Death of Massive Stars: Supernovae and Gamma-Ray Bursts , April 2011 , pp. 40 - 45
Copyright
Copyright © International Astronomical Union 2012

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