Search for first harmonic modulation in the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory

Autores
Dova, María Teresa; Gómez Albarracín, Flavia Alejandra; Hansen, Patricia María; Mariazzi, Analisa Gabriela; Moreno, Juan Cruz; Sciutto, Sergio Juan; Wahlberg, Hernán Pablo; The Pierre Auger Collaboration
Año de publicación
2010
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present the results of searches for dipolar-type anisotropies in different energy ranges above 2.5 x 1017 eV with the surface detector array of the Pierre Auger Observatory, reporting on both the phase and the amplitude measurements of the first harmonic modulation in the right-ascension distribution. Upper limits on the amplitudes are obtained, which provide the most stringent bounds at present, being below 2% at 99% C.L. for EeV energies. We also compare our results to those of previous experiments as well as with some theoretical expectations.
Facultad de Ciencias Exactas
Materia
Ciencias Exactas
Física
Radiación cósmica
Anisotropía
Pierre Auger Observatory
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/80660

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network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling Search for first harmonic modulation in the right ascension distribution of cosmic rays detected at the Pierre Auger ObservatoryDova, María TeresaGómez Albarracín, Flavia AlejandraHansen, Patricia MaríaMariazzi, Analisa GabrielaMoreno, Juan CruzSciutto, Sergio JuanWahlberg, Hernán PabloThe Pierre Auger CollaborationCiencias ExactasFísicaRadiación cósmicaAnisotropíaPierre Auger ObservatoryWe present the results of searches for dipolar-type anisotropies in different energy ranges above 2.5 x 10<sup>17</sup> eV with the surface detector array of the Pierre Auger Observatory, reporting on both the phase and the amplitude measurements of the first harmonic modulation in the right-ascension distribution. Upper limits on the amplitudes are obtained, which provide the most stringent bounds at present, being below 2% at 99% C.L. for EeV energies. We also compare our results to those of previous experiments as well as with some theoretical expectations.Facultad de Ciencias Exactas2010-12-28info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf627-639http://sedici.unlp.edu.ar/handle/10915/80660enginfo:eu-repo/semantics/altIdentifier/issn/0927-6505info:eu-repo/semantics/altIdentifier/doi/10.1016/j.astropartphys.2010.12.007info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-03T10:47:08Zoai:sedici.unlp.edu.ar:10915/80660Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-03 10:47:09.143SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Search for first harmonic modulation in the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory
title Search for first harmonic modulation in the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory
spellingShingle Search for first harmonic modulation in the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory
Dova, María Teresa
Ciencias Exactas
Física
Radiación cósmica
Anisotropía
Pierre Auger Observatory
title_short Search for first harmonic modulation in the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory
title_full Search for first harmonic modulation in the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory
title_fullStr Search for first harmonic modulation in the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory
title_full_unstemmed Search for first harmonic modulation in the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory
title_sort Search for first harmonic modulation in the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory
dc.creator.none.fl_str_mv Dova, María Teresa
Gómez Albarracín, Flavia Alejandra
Hansen, Patricia María
Mariazzi, Analisa Gabriela
Moreno, Juan Cruz
Sciutto, Sergio Juan
Wahlberg, Hernán Pablo
The Pierre Auger Collaboration
author Dova, María Teresa
author_facet Dova, María Teresa
Gómez Albarracín, Flavia Alejandra
Hansen, Patricia María
Mariazzi, Analisa Gabriela
Moreno, Juan Cruz
Sciutto, Sergio Juan
Wahlberg, Hernán Pablo
The Pierre Auger Collaboration
author_role author
author2 Gómez Albarracín, Flavia Alejandra
Hansen, Patricia María
Mariazzi, Analisa Gabriela
Moreno, Juan Cruz
Sciutto, Sergio Juan
Wahlberg, Hernán Pablo
The Pierre Auger Collaboration
author2_role author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Ciencias Exactas
Física
Radiación cósmica
Anisotropía
Pierre Auger Observatory
topic Ciencias Exactas
Física
Radiación cósmica
Anisotropía
Pierre Auger Observatory
dc.description.none.fl_txt_mv We present the results of searches for dipolar-type anisotropies in different energy ranges above 2.5 x 10<sup>17</sup> eV with the surface detector array of the Pierre Auger Observatory, reporting on both the phase and the amplitude measurements of the first harmonic modulation in the right-ascension distribution. Upper limits on the amplitudes are obtained, which provide the most stringent bounds at present, being below 2% at 99% C.L. for EeV energies. We also compare our results to those of previous experiments as well as with some theoretical expectations.
Facultad de Ciencias Exactas
description We present the results of searches for dipolar-type anisotropies in different energy ranges above 2.5 x 10<sup>17</sup> eV with the surface detector array of the Pierre Auger Observatory, reporting on both the phase and the amplitude measurements of the first harmonic modulation in the right-ascension distribution. Upper limits on the amplitudes are obtained, which provide the most stringent bounds at present, being below 2% at 99% C.L. for EeV energies. We also compare our results to those of previous experiments as well as with some theoretical expectations.
publishDate 2010
dc.date.none.fl_str_mv 2010-12-28
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://sedici.unlp.edu.ar/handle/10915/80660
url http://sedici.unlp.edu.ar/handle/10915/80660
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/0927-6505
info:eu-repo/semantics/altIdentifier/doi/10.1016/j.astropartphys.2010.12.007
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.format.none.fl_str_mv application/pdf
627-639
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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