Gamma-Ray Burst Follow-up Observations with STACEE During 2003-2007

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dc.creatorSTACEE Collaboration
dc.creatorJarvis, A.
dc.creatorBall, J.
dc.creatorCarson, J. E.
dc.creatorCovault, C. E.
dc.creatorDriscoll, D. D.
dc.creatorFortin, P.
dc.creatorGingrich, D. M.
dc.creatorHanna, D. S.
dc.creatorKildea, J.
dc.creatorLindner, T.
dc.creatorMukherjee, R.
dc.creatorMueller, C.
dc.creatorOng, R. A.
dc.creatorRagan, K.
dc.creatorWilliams, D. A.
dc.creatorZweerink, J.
dc.date2007-10-22
dc.date.accessioned2026-07-07T08:37:52Z
dc.date.available2026-07-07T08:37:52Z
dc.descriptionThe Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE) is an atmospheric Cherenkov telescope (ACT) that uses a large mirror array to achieve a relatively low energy threshold. For sources with Crab-like spectra, at high elevations, the detector response peaks near 100 GeV. Gamma-ray burst (GRB) observations have been a high priority for the STACEE collaboration since the inception of the experiment. We present the results of 20 GRB follow-up observations at times ranging from 3 minutes to 15 hours after the burst triggers. Where redshift measurements are available, we place constraints on the intrinsic high-energy spectra of the bursts.
dc.description4 pages, 1 table, 2 figures, presented at the 30th International Cosmic Ray Conference, Merida, Mexico, 2007
dc.identifierhttps://arxiv.org/abs/0710.4149
dc.identifierhttp://arxiv.org/abs/0710.4149
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/140553
dc.subjectAstrophysics
dc.titleGamma-Ray Burst Follow-up Observations with STACEE During 2003-2007
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