par Abraham, Jared D.;Maris, Ioana Codrina
; [et al.]
Référence Astroparticle physics, 31, 6, page (399-406)
Publication Publié, 2009

Référence Astroparticle physics, 31, 6, page (399-406)
Publication Publié, 2009
Article révisé par les pairs
Résumé : | From direct observations of the longitudinal development of ultra-high energy air showers performed with the Pierre Auger Observatory, upper limits of 3.8%, 2.4%, 3.5% and 11.7% (at 95% c.l.) are obtained on the fraction of cosmic-ray photons above 2, 3, 5 and 10 EeV (1 EeV ≡ 1018 eV), respectively. These are the first experimental limits on ultra-high energy photons at energies below 10 EeV. The results complement previous constraints on top-down models from array data and they reduce systematic uncertainties in the interpretation of shower data in terms of primary flux, nuclear composition and proton-air cross-section. © 2009 Elsevier B.V. All rights reserved. |