Primary Energy Spectra and Elemental Composition. GAMMA Experiment

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dc.creatorTer-Antonyan, S. V.
dc.creatorMartirosov, R. M.
dc.creatorGaryaka, A. P.
dc.creatorEganov, V.
dc.creatorNikolskaya, N.
dc.creatorEpiskoposyan, T.
dc.creatorProcureur, J.
dc.creatorGallant, Y.
dc.creatorJones, L.
dc.date2005-06-24
dc.date.accessioned2026-07-07T02:18:04Z
dc.date.available2026-07-07T02:18:04Z
dc.descriptionOn the basis of the Extensive Air Shower data observed by the GAMMA experiment the energy spectra and elemental composition of the primary cosmic rays have been derived in the 1-100 PeV energy range. Reconstruction of the primary energy spectra is carried out in the framework of the SIBYLL and QGSJET interaction models and the hypothesis of the power-law steepening primary energy spectra. All presented results are derived taking into account the detector response, reconstruction uncertainties of EAS parameters and fluctuation of EAS development.
dc.description11 pages, 14 figures, submitted to 29th International Cosmic Ray Conference, Pune
dc.identifierhttps://arxiv.org/abs/astro-ph/0506588
dc.identifierhttp://arxiv.org/abs/astro-ph/0506588
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9352
dc.subjectAstrophysics
dc.titlePrimary Energy Spectra and Elemental Composition. GAMMA Experiment
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