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GRB Prompt X-ray Emission

Published online by Cambridge University Press:  05 September 2012

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: [email protected]
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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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

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