The Role of the BATSE Instrument Response in Creating the Gamma-Ray Burst E-Peak Distribution

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dc.creatorBrainerd, J. J.
dc.creatorPendleton, G.
dc.creatorMallozzi, R.
dc.creatorBriggs, M. S.
dc.creatorPreece, R. D.
dc.date1999-04-02
dc.date.accessioned2026-07-07T02:31:07Z
dc.date.available2026-07-07T02:31:07Z
dc.descriptionAll gamma-ray bursts are observed to have approximately the same characteristic gamma-ray energy. We show in this article that for bursts in the BATSE data set, this property as measured by the E-peak value is not an instrumental effect, but a physical property of gamma-ray bursts.
dc.descriptionPresented at the 20 Texas Symposium on Relativistic Astrophysics, December 1998, Paris, France. To appear on the proceedings compact disk
dc.identifierhttps://arxiv.org/abs/astro-ph/9904039
dc.identifierhttp://arxiv.org/abs/astro-ph/9904039
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14047
dc.subjectAstrophysics
dc.titleThe Role of the BATSE Instrument Response in Creating the Gamma-Ray Burst E-Peak Distribution
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