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Upper limit on the cosmic-ray photon fraction at EeV energies from the Pierre Auger Observatory

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dc.contributor.author Abraham, J.
dc.contributor.author Pepe, Iuri Muniz
dc.contributor.author Abreu, P.
dc.contributor.author Aglietta, M.
dc.contributor.author Aguirre, C.
dc.contributor.author Ahn, E. J.
dc.creator Abraham, J.
dc.creator Pepe, Iuri Muniz
dc.creator Abreu, P.
dc.creator Aglietta, M.
dc.creator Aguirre, C.
dc.creator Ahn, E. J.
dc.date.accessioned 2013-11-19T20:24:56Z
dc.date.issued 2009
dc.identifier.issn 0927-6505
dc.identifier.uri http://repositorio.ufba.br/ri/handle/ri/13777
dc.description Texto completo: acesso restrito. p. 399–406 pt_BR
dc.description.abstract 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 View the MathML source, 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. pt_BR
dc.language.iso en pt_BR
dc.rights Acesso Aberto pt_BR
dc.source http://dx.doi.org/10.1016/j.astropartphys.2009.04.003 pt_BR
dc.title Upper limit on the cosmic-ray photon fraction at EeV energies from the Pierre Auger Observatory pt_BR
dc.title.alternative Astroparticle Physics pt_BR
dc.type Artigo de Periódico pt_BR
dc.identifier.number v. 31, n. 6 pt_BR
dc.embargo.liftdate 10000-01-01


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