Search for TeV Counterparts in Gamma-Ray Bursts

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dc.creatorBoyle, P. J.
dc.creatorBuckley, J. H.
dc.creatorBurdett, A. M.
dc.creatorGordo, J. Bussons
dc.creatorCarter-Lewis, D. A.
dc.creatorCatanese, M.
dc.creatorCawley, M. F.
dc.creatorConnaughton, V.
dc.creatorFegan, D. J.
dc.creatorFinley, J. P.
dc.creatorGaidos, J. A.
dc.creatorHarris, K.
dc.creatorHillas, A. M.
dc.creatorLamb, R. C.
dc.creatorKrennrich, F.
dc.creatorLessard, R. W.
dc.creatorMasterson, C.
dc.creatorMcEnery, J. E.
dc.creatorMohanty, G.
dc.creatorPorter, N. A.
dc.creatorQuinn, J.
dc.creatorRodgers, A. J.
dc.creatorRose, H. J.
dc.creatorSamuelson, F. W.
dc.creatorSembroski, G. H.
dc.creatorSrinivasan, R.
dc.creatorWeekes, T. C.
dc.creatorZweerink, J.
dc.date1997-06-13
dc.date.accessioned2026-07-07T02:23:36Z
dc.date.available2026-07-07T02:23:36Z
dc.descriptionBased on BACODINE network notification the Whipple Observatory gamma-ray telescope has been used to search for the delayed TeV counterpart to BATSE-detected gamma-ray bursts. In the fast slew mode, any point in the sky can be reached within two minutes of the burst notification. The search strategy, necessary because of the uncertainty in burst position and limited FOV of the camera, is described.
dc.description4 pages, 3 figures, to appear in proceedings of the 25th ICRC (Durban)
dc.identifierhttps://arxiv.org/abs/astro-ph/9706132
dc.identifierhttp://arxiv.org/abs/astro-ph/9706132
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11306
dc.subjectAstrophysics
dc.titleSearch for TeV Counterparts in Gamma-Ray Bursts
dc.typetext

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