Auteur(s): Ter-Antonyan S. V., Martirosov R. M., Garyaka A. P., Eganov V., Nikolskaya N., Episkoposyan T., Procureur J., Gallant Y., Jones L.
(Document sans référence bibliographique) 2005-06-24Texte intégral en Openaccess : 
Ref HAL: hal-00430451_v1
Ref Arxiv: astro-ph/0506588
Ref. & Cit.: NASA ADS
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Résumé:
On 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.
Commentaires: 11 pages, 14 figures, submitted to 29th International Cosmic Ray Conference, Pune