%0 Unpublished work
%T Primary Energy Spectra and Elemental Composition. GAMMA Experiment
%+ Laboratoire de Physique Théorique et Astroparticules (LPTA)
%A Ter-Antonyan, S. V.
%A Martirosov, R. M.
%A Garyaka, A. P.
%A Eganov, V.
%A Nikolskaya, N.
%A Episkoposyan, T.
%A Procureur, J.
%A Gallant, Yves
%A Jones, L.
%Z 11 pages, 14 figures, submitted to 29th International Cosmic Ray Conference, Pune
%Z 05-045
%8 2005-06-24
%D 2005
%Z astro-ph/0506588
%Z Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]
%Z Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Preprints, Working Papers, ...
%X 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.
%G English
%L hal-00430451
%U https://hal.science/hal-00430451
%~ IN2P3
%~ LPTA
%~ CNRS
%~ UNIV-MONTP2
%~ UNIV-MONTPELLIER
%~ UM1-UM2