Gamma ray bursts at high energies : detection ranges and event rates

dc.contributor.author	Shanthi, K
dc.contributor.author	Kaul, C. L
dc.contributor.author	Kaul, R. K
dc.contributor.author	Tickoo, A. K
dc.contributor.author	Bhat, C. L
dc.date.accessioned	2008-06-20T08:03:10Z
dc.date.available	2008-06-20T08:03:10Z
dc.date.issued	2002
dc.identifier.citation	BASI, Vol. 30, No. 1, pp. 429 - 434	en
dc.identifier.uri	http://hdl.handle.net/2248/2475
dc.description.abstract	The Gamma-Ray Burst (GRB) detection rates at energies ? 20GeV, have been estimated for the 3 atmospheric Cerenkov telescope systems of the GRACE project at Mt. Abu, under the assumption that the bursts have a cosmological origin and a continuous power-law spectrum in the MeV-TeV energy range. The attention of high energy gamma-ray photons in a burst, during its propagation in the intergalactic space, has ben taken into account by assuming two extreme scenarios of the Extragalactic Background Radiation (EBR) fields.	en
dc.format.extent	553496 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2002BASI...30..429S	en
dc.subject	Gamma Ray Bursts	en
dc.subject	High Energy Tails	en
dc.subject	Detection Range	en
dc.subject	Event Rate	en
dc.title	Gamma ray bursts at high energies : detection ranges and event rates	en
dc.type	Article	en