Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2475
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dc.contributor.authorShanthi, K-
dc.contributor.authorKaul, C. L-
dc.contributor.authorKaul, R. K-
dc.contributor.authorTickoo, A. K-
dc.contributor.authorBhat, C. L-
dc.date.accessioned2008-06-20T08:03:10Z-
dc.date.available2008-06-20T08:03:10Z-
dc.date.issued2002-
dc.identifier.citationBASI, Vol. 30, No. 1, pp. 429 - 434en
dc.identifier.urihttp://hdl.handle.net/2248/2475-
dc.description.abstractThe 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.extent553496 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2002BASI...30..429Sen
dc.subjectGamma Ray Burstsen
dc.subjectHigh Energy Tailsen
dc.subjectDetection Rangeen
dc.subjectEvent Rateen
dc.titleGamma ray bursts at high energies : detection ranges and event ratesen
dc.typeArticleen
Appears in Collections:BASI Publications

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