Search for GeV GRBs with the INCA experiment

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dc.contributor.authorRenán Cabrera
dc.contributor.authorA. Castellina
dc.contributor.authorP. L. Ghia
dc.contributor.authorF. Kakimoto
dc.contributor.authorT. Kaneko
dc.contributor.authorC. Morello
dc.contributor.authorG. Navarra
dc.contributor.authorK. Nishi
dc.contributor.authorO. Saavedra
dc.contributor.authorG. Trinchero
dc.coverage.spatialBolivia
dc.date.accessioned2026-03-22T15:23:45Z
dc.date.available2026-03-22T15:23:45Z
dc.date.issued1999
dc.descriptionCitaciones: 8
dc.description.abstractINCA is an air shower array located at Mount Chacaltaya in Bolivia, at 5200 m a.s.l., searching for Gamma Ray Bursts of energy GeV. The results presented here concern a GRB search made in correlation with 70 events recorded by BATSE since December 1996 to August 1998. For every burst, the INCA counting rate has been studied both during the BATSE detection time and in 2 hours around. No significant excess has been found in any of the trials. Assuming for the burst a power low energy spectrum extending up to 1 TeV with a slope and a time duration of 10 s, the obtained energy fluence upper limits range from to depending on the event zenith angle.
dc.identifier.doi10.1051/aas:1999368
dc.identifier.urihttps://doi.org/10.1051/aas:1999368
dc.identifier.urihttps://andeanlibrary.org/handle/123456789/52119
dc.language.isoen
dc.publisherEDP Sciences
dc.relation.ispartofAstronomy and Astrophysics Supplement Series
dc.sourceHigher University of San Andrés
dc.subjectGamma-ray burst
dc.subjectZenith
dc.subjectPhysics
dc.subjectAir shower
dc.subjectAstrophysics
dc.subjectRange (aeronautics)
dc.subjectFluence
dc.subjectEnergy (signal processing)
dc.subjectEvent (particle physics)
dc.subjectEnergy spectrum
dc.titleSearch for GeV GRBs with the INCA experiment
dc.typearticle

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