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Poster communications

Upper bound on the flux of cosmic photons and neutrinos of ultra-high energy with the Pierre AUGER Observatory

Abstract : The Pierre Auger Observatory detects the atmospheric showers induced by ultra-energetic cosmic rays. Photons or neutrinos may be clearly distinguished from protons or nuclei. The discriminating features are described; upper bounds to the incident fluxes are extracted from the data taken during the first two years of operation of the Observatory, and compared to theoretical models.
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http://hal.in2p3.fr/in2p3-00171061
Contributor : Dominique Girod <>
Submitted on : Tuesday, September 11, 2007 - 2:10:52 PM
Last modification on : Friday, April 10, 2020 - 5:31:04 PM

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  • HAL Id : in2p3-00171061, version 1

Citation

P. Billoir. Upper bound on the flux of cosmic photons and neutrinos of ultra-high energy with the Pierre AUGER Observatory. Semaine de l'Astrophysique Française (SF2A 2007), Jul 2007, Grenoble, France. Société Française d'Astronomie et d'Astrophysique, à paraitre, 2007. ⟨in2p3-00171061⟩

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