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Measurement of the cosmic ray spectrum above 4×10^<SUP>18</SUP> eV using inclined events detected with the Pierre Auger Observatory

By María Teresa Dova, Patricia María Hansen, Cecilia Gisele Jarne, Analisa Gabriela Mariazzi, Sergio Juan Sciutto, Hernán Pablo Wahlberg and The Pierre Auger Collaboration


A measurement of the cosmic-ray spectrum for energies exceeding 4×1018 eVis presented, which is based on the analysis of showers with zenith angles greater than60◦ detected with the Pierre Auger Observatory between 1 January 2004 and 31 December 2013. The measured spectrum confirms a flux suppression at the highest energies.Above 5.3×1018 eV, the ?ankle?, the flux can be described by a power law E −γ with index γ = 2.70 ± 0.02 (stat) ± 0.1 (sys) followed by a smooth suppression region. For the energy(Es ) at which the spectral flux has fallen to one-half of its extrapolated value in the absence of suppression, we find Es = (5.12 ± 0.25 (stat)−1.2 (sys))×10 eV.La nómina completa de autores puede accederse al final del documento asociado a este ítem.Instituto de Física La PlataConsejo Nacional de Investigaciones Científicas y Técnica

Topics: Física
Year: 2014
DOI identifier: 10.1088/1475-7516/2015/08/049/meta
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