The Pierre Auger Cosmic Ray Observatory

Autores
Dova, María Teresa; Martínez, Nora; Mariazzi, Analisa Gabriela; Wahlberg, Hernán Pablo; The Pierre Auger Collaboration
Año de publicación
2015
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The Pierre Auger Observatory, located on a vast, high plain in western Argentina, is the world's largest cosmic ray observatory. The objectives of the Observatory are to probe the origin and characteristics of cosmic rays above 1017 eV and to study the interactions of these, the most energetic particles observed in nature. The Auger design features an array of 1660 water Cherenkov particle detector stations spread over 3000 km2 overlooked by 24 air fluorescence telescopes. In addition, three high elevation fluorescence telescopes overlook a 23.5 km2 , 61-detector infilled array with 750 m spacing. The Observatory has been in successful operation since completion in 2008 and has recorded data from an exposure exceeding 40,000 km2 sr yr. This paper describes the design and performance of the detectors, related subsystems and infrastructure that make up the Observatory.
Facultad de Ciencias Exactas
Materia
Ciencias Exactas
Física
Pierre Auger Observatory
high energy cosmic rays
hybrid observatory
water Cherenkov detectors
air fluorescence detectors
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:10915/75102

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network_name_str SEDICI (UNLP)
spelling The Pierre Auger Cosmic Ray ObservatoryDova, María TeresaMartínez, NoraMariazzi, Analisa GabrielaWahlberg, Hernán PabloThe Pierre Auger CollaborationCiencias ExactasFísicaPierre Auger Observatoryhigh energy cosmic rayshybrid observatorywater Cherenkov detectorsair fluorescence detectorsThe Pierre Auger Observatory, located on a vast, high plain in western Argentina, is the world's largest cosmic ray observatory. The objectives of the Observatory are to probe the origin and characteristics of cosmic rays above 1017 eV and to study the interactions of these, the most energetic particles observed in nature. The Auger design features an array of 1660 water Cherenkov particle detector stations spread over 3000 km2 overlooked by 24 air fluorescence telescopes. In addition, three high elevation fluorescence telescopes overlook a 23.5 km2 , 61-detector infilled array with 750 m spacing. The Observatory has been in successful operation since completion in 2008 and has recorded data from an exposure exceeding 40,000 km2 sr yr. This paper describes the design and performance of the detectors, related subsystems and infrastructure that make up the Observatory.Facultad de Ciencias Exactas2015-07-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf172-213http://sedici.unlp.edu.ar/handle/10915/75102enginfo:eu-repo/semantics/altIdentifier/issn/0168-9002info:eu-repo/semantics/altIdentifier/doi/10.1016/j.nima.2015.06.058info: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:UNLP2025-09-03T10:44:12Zoai:sedici.unlp.edu.ar:10915/75102Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-03 10:44:12.983SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv The Pierre Auger Cosmic Ray Observatory
title The Pierre Auger Cosmic Ray Observatory
spellingShingle The Pierre Auger Cosmic Ray Observatory
Dova, María Teresa
Ciencias Exactas
Física
Pierre Auger Observatory
high energy cosmic rays
hybrid observatory
water Cherenkov detectors
air fluorescence detectors
title_short The Pierre Auger Cosmic Ray Observatory
title_full The Pierre Auger Cosmic Ray Observatory
title_fullStr The Pierre Auger Cosmic Ray Observatory
title_full_unstemmed The Pierre Auger Cosmic Ray Observatory
title_sort The Pierre Auger Cosmic Ray Observatory
dc.creator.none.fl_str_mv Dova, María Teresa
Martínez, Nora
Mariazzi, Analisa Gabriela
Wahlberg, Hernán Pablo
The Pierre Auger Collaboration
author Dova, María Teresa
author_facet Dova, María Teresa
Martínez, Nora
Mariazzi, Analisa Gabriela
Wahlberg, Hernán Pablo
The Pierre Auger Collaboration
author_role author
author2 Martínez, Nora
Mariazzi, Analisa Gabriela
Wahlberg, Hernán Pablo
The Pierre Auger Collaboration
author2_role author
author
author
author
dc.subject.none.fl_str_mv Ciencias Exactas
Física
Pierre Auger Observatory
high energy cosmic rays
hybrid observatory
water Cherenkov detectors
air fluorescence detectors
topic Ciencias Exactas
Física
Pierre Auger Observatory
high energy cosmic rays
hybrid observatory
water Cherenkov detectors
air fluorescence detectors
dc.description.none.fl_txt_mv The Pierre Auger Observatory, located on a vast, high plain in western Argentina, is the world's largest cosmic ray observatory. The objectives of the Observatory are to probe the origin and characteristics of cosmic rays above 1017 eV and to study the interactions of these, the most energetic particles observed in nature. The Auger design features an array of 1660 water Cherenkov particle detector stations spread over 3000 km2 overlooked by 24 air fluorescence telescopes. In addition, three high elevation fluorescence telescopes overlook a 23.5 km2 , 61-detector infilled array with 750 m spacing. The Observatory has been in successful operation since completion in 2008 and has recorded data from an exposure exceeding 40,000 km2 sr yr. This paper describes the design and performance of the detectors, related subsystems and infrastructure that make up the Observatory.
Facultad de Ciencias Exactas
description The Pierre Auger Observatory, located on a vast, high plain in western Argentina, is the world's largest cosmic ray observatory. The objectives of the Observatory are to probe the origin and characteristics of cosmic rays above 1017 eV and to study the interactions of these, the most energetic particles observed in nature. The Auger design features an array of 1660 water Cherenkov particle detector stations spread over 3000 km2 overlooked by 24 air fluorescence telescopes. In addition, three high elevation fluorescence telescopes overlook a 23.5 km2 , 61-detector infilled array with 750 m spacing. The Observatory has been in successful operation since completion in 2008 and has recorded data from an exposure exceeding 40,000 km2 sr yr. This paper describes the design and performance of the detectors, related subsystems and infrastructure that make up the Observatory.
publishDate 2015
dc.date.none.fl_str_mv 2015-07-08
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/10915/75102
url http://sedici.unlp.edu.ar/handle/10915/75102
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/0168-9002
info:eu-repo/semantics/altIdentifier/doi/10.1016/j.nima.2015.06.058
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
172-213
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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