Large scale distribution of ultra high energy cosmic rays detected at the Pierre Auger observatory with zenith angles up to 80 °

We present the results of an analysis of the large angular scale distribution of the arrival directions of cosmic rays with energy above 4 EeV detected at the Pierre Auger Observatory including for the first time events with zenith angle between 60° and 80°. We perform two Rayleigh analyses, one in...

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Publicado: 2015
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Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v802_n2_p_Multitudinario
http://hdl.handle.net/20.500.12110/paper_0004637X_v802_n2_p_Multitudinario
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spelling paper:paper_0004637X_v802_n2_p_Multitudinario2023-06-08T14:29:14Z Large scale distribution of ultra high energy cosmic rays detected at the Pierre Auger observatory with zenith angles up to 80 ° Astroparticle physics Cosmic rays We present the results of an analysis of the large angular scale distribution of the arrival directions of cosmic rays with energy above 4 EeV detected at the Pierre Auger Observatory including for the first time events with zenith angle between 60° and 80°. We perform two Rayleigh analyses, one in the right ascension and one in the azimuth angle distributions, that are sensitive to modulations in right ascension and declination, respectively. The largest departure from isotropy appears in the 98 E > 8 EeV energy bin, with an amplitude for the first harmonic in right ascension r 1 α = (4.4 ± 1.0) × 10 -2 , that has a chance probability P (≥ 1 α ) = 6.4 × 10 -5 , reinforcing the hint previously reported with vertical events alone. © 2015, The American Astronomical Society. All rights reserved. 2015 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v802_n2_p_Multitudinario http://hdl.handle.net/20.500.12110/paper_0004637X_v802_n2_p_Multitudinario
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Astroparticle physics
Cosmic rays
spellingShingle Astroparticle physics
Cosmic rays
Large scale distribution of ultra high energy cosmic rays detected at the Pierre Auger observatory with zenith angles up to 80 °
topic_facet Astroparticle physics
Cosmic rays
description We present the results of an analysis of the large angular scale distribution of the arrival directions of cosmic rays with energy above 4 EeV detected at the Pierre Auger Observatory including for the first time events with zenith angle between 60° and 80°. We perform two Rayleigh analyses, one in the right ascension and one in the azimuth angle distributions, that are sensitive to modulations in right ascension and declination, respectively. The largest departure from isotropy appears in the 98 E > 8 EeV energy bin, with an amplitude for the first harmonic in right ascension r 1 α = (4.4 ± 1.0) × 10 -2 , that has a chance probability P (≥ 1 α ) = 6.4 × 10 -5 , reinforcing the hint previously reported with vertical events alone. © 2015, The American Astronomical Society. All rights reserved.
title Large scale distribution of ultra high energy cosmic rays detected at the Pierre Auger observatory with zenith angles up to 80 °
title_short Large scale distribution of ultra high energy cosmic rays detected at the Pierre Auger observatory with zenith angles up to 80 °
title_full Large scale distribution of ultra high energy cosmic rays detected at the Pierre Auger observatory with zenith angles up to 80 °
title_fullStr Large scale distribution of ultra high energy cosmic rays detected at the Pierre Auger observatory with zenith angles up to 80 °
title_full_unstemmed Large scale distribution of ultra high energy cosmic rays detected at the Pierre Auger observatory with zenith angles up to 80 °
title_sort large scale distribution of ultra high energy cosmic rays detected at the pierre auger observatory with zenith angles up to 80 °
publishDate 2015
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v802_n2_p_Multitudinario
http://hdl.handle.net/20.500.12110/paper_0004637X_v802_n2_p_Multitudinario
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