Searches for anisotropies in the arrival directions of the highest energy cosmic rays detected by the Pierre Auger Observatory

We analyze the distribution of arrival directions of ultra-high-energy cosmic rays recorded at the Pierre Auger Observatory in 10 years of operation. The data set, about three times larger than that used in earlier studies, includes arrival directions with zenith angles up to 80°, thus covering from...

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Detalles Bibliográficos
Autores principales: Dova, María Teresa, Hansen, Patricia María, Jarne, Cecilia Gisele, Mariazzi, Analisa Gabriela, Sciutto, Sergio Juan, The Pierre Auger Collaboration
Formato: Articulo
Lenguaje:Inglés
Publicado: 2015
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/72993
Aporte de:
id I19-R120-10915-72993
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Exactas
Física
acceleration of particles; astroparticle physics
spellingShingle Ciencias Exactas
Física
acceleration of particles; astroparticle physics
Dova, María Teresa
Hansen, Patricia María
Jarne, Cecilia Gisele
Mariazzi, Analisa Gabriela
Sciutto, Sergio Juan
The Pierre Auger Collaboration
Searches for anisotropies in the arrival directions of the highest energy cosmic rays detected by the Pierre Auger Observatory
topic_facet Ciencias Exactas
Física
acceleration of particles; astroparticle physics
description We analyze the distribution of arrival directions of ultra-high-energy cosmic rays recorded at the Pierre Auger Observatory in 10 years of operation. The data set, about three times larger than that used in earlier studies, includes arrival directions with zenith angles up to 80°, thus covering from -90º to +45º in declination. After updating the fraction of events correlating with the active galactic nuclei (AGNs) in the Véron-Cetty and Véron catalog, we subject the arrival directions of the data with energies in excess of 40 EeV to different tests for anisotropy. We search for localized excess fluxes, self-clustering of event directions at angular scales up to 30°, and different threshold energies between 40 and 80 EeV. We then look for correlations of cosmic rays with celestial structures both in the Galaxy (the Galactic Center and Galactic Plane) and in the local universe (the Super-Galactic Plane). We also examine their correlation with different populations of nearby extragalactic objects: galaxies in the 2MRS catalog, AGNs detected by Swift-BAT, radio galaxies with jets, and the Centaurus A (Cen A) galaxy. None of the tests show statistically significant evidence of anisotropy. The strongest departures from isotropy (post-trial probability ~1.4%) are obtained for cosmic rays with E > 58 EeV in rather large windows around Swift AGNs closer than 130 Mpc and brighter than 1044 erg s−1 (18° radius), and around the direction of Cen A (15° radius).
format Articulo
Articulo
author Dova, María Teresa
Hansen, Patricia María
Jarne, Cecilia Gisele
Mariazzi, Analisa Gabriela
Sciutto, Sergio Juan
The Pierre Auger Collaboration
author_facet Dova, María Teresa
Hansen, Patricia María
Jarne, Cecilia Gisele
Mariazzi, Analisa Gabriela
Sciutto, Sergio Juan
The Pierre Auger Collaboration
author_sort Dova, María Teresa
title Searches for anisotropies in the arrival directions of the highest energy cosmic rays detected by the Pierre Auger Observatory
title_short Searches for anisotropies in the arrival directions of the highest energy cosmic rays detected by the Pierre Auger Observatory
title_full Searches for anisotropies in the arrival directions of the highest energy cosmic rays detected by the Pierre Auger Observatory
title_fullStr Searches for anisotropies in the arrival directions of the highest energy cosmic rays detected by the Pierre Auger Observatory
title_full_unstemmed Searches for anisotropies in the arrival directions of the highest energy cosmic rays detected by the Pierre Auger Observatory
title_sort searches for anisotropies in the arrival directions of the highest energy cosmic rays detected by the pierre auger observatory
publishDate 2015
url http://sedici.unlp.edu.ar/handle/10915/72993
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