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
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/75102
Ver los metadatos del registro completo
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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) |
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openAccess |
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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 |
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