Authors

A. Aab, Universität SiegenFollow
P. Abreu, Universidade de LisboaFollow
M. Aglietta, Università degli Studi di TorinoFollow
E. J. Ahn, Fermi National Accelerator LaboratoryFollow
I. Al Samarai, Institut de Physique Nucléaire d’Orsay
I. F.M. Albuquerque, Universidade de São PauloFollow
I. Allekotte, Centro Atomico BarilocheFollow
J. Allen, New York UniversityFollow
P. Allison, The Ohio State UniversityFollow
A. Almela, Universidad Nacional de San Martín
J. Alvarez Castillo, Universidad Nacional Autónoma de México
J. Alvarez-Muñiz, Universidad de Santiago de CompostelaFollow
R. Alves Batista, Universität Hamburg
M. Ambrosio, Università degli Studi di Napoli Federico IIFollow
A. Aminaei, Radboud UniversiteitFollow
L. Anchordoqui, City University of New YorkFollow
S. Andringa, Universidade de LisboaFollow
C. Aramo, Università degli Studi di Napoli Federico II
V. M. Aranda, Universidad Complutense de Madrid
F. Arqueros, Universidad Complutense de Madrid
H. Asorey, Centro Atomico Bariloche
P. Assis, Universidade de Lisboa
J. Aublin, Laboratoire de Physique Nucléaire et de Hautes Energies
M. Ave, Universidad de Santiago de Compostela
M. Avenier, Universite Grenoble Alpes
G. Avila, Pierre Auger Observatory
N. Awal, New York University
A. M. Badescu, University Politehnica of Bucharest
K. B. Barber, The University of Adelaide
J. Bäuml, Karlsruher Institut für Technologie, Campus Süd
C. Baus, Karlsruher Institut für Technologie, Campus Süd
J. J. Beatty, The Ohio State University
K. H. Becker, Bergische Universität Wuppertal

Document Type

Article

Publication Date

6-23-2015

Abstract

Energy-dependent patterns in the arrival directions of cosmic rays are searched for using data of the Pierre Auger Observatory. We investigate local regions around the highest-energy cosmic rays with E ≥ 6×1019 eV by analyzing cosmic rays with energies above E ≥ 5×1018 eV arriving within an angular separation of approximately 15. We characterize the energy distributions inside these regions by two independent methods, one searching for angular dependence of energy-energy correlations and one searching for collimation of energy along the local system of principal axes of the energy distribution. No significant patterns are found with this analysis. The comparison of these measurements with astrophysical scenarios can therefore be used to obtain constraints on related model parameters such as strength of cosmic-ray deflection and density of point sources.

Publication Source (Journal or Book title)

European Physical Journal C

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