Properties and performance of the prototype instrument for the Pierre Auger Observatory
- Autores
- Cillis, Analía Nilda; Dova, María Teresa; Epele, Luis Nicolás; Grunfeld, Christian Martín; Manceñido, Mónica E.; Mariazzi, Analisa Gabriela; Martínez, Nora; Sciutto, Sergio Juan; Veiga, Alejandro Luis; The Pierre Auger Collaboration
- Año de publicación
- 2004
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Construction of the first stage of the Pierre Auger Observatory has begun. The aim of the Observatory is to collect unprecedented information about cosmic rays above 10^18 eV. The first phase of the project, the construction and operation of a prototype system, known as the engineering array, has now been completed. It has allowed all of the sub-systems that will be used in the full instrument to be tested under field conditions. In this paper, the properties and performance of these sub-systems are described and their success illustrated with descriptions of some of the events recorded thus far.
La lista completa de autores puede verse en el archivo asociado.
Facultad de Ciencias Exactas - Materia
-
Física
Prototype instrument
Pierre Auger Observatory
Cosmic rays - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/78286
Ver los metadatos del registro completo
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Properties and performance of the prototype instrument for the Pierre Auger ObservatoryCillis, Analía NildaDova, María TeresaEpele, Luis NicolásGrunfeld, Christian MartínManceñido, Mónica E.Mariazzi, Analisa GabrielaMartínez, NoraSciutto, Sergio JuanVeiga, Alejandro LuisThe Pierre Auger CollaborationFísicaPrototype instrumentPierre Auger ObservatoryCosmic raysConstruction of the first stage of the Pierre Auger Observatory has begun. The aim of the Observatory is to collect unprecedented information about cosmic rays above 10^18 eV. The first phase of the project, the construction and operation of a prototype system, known as the engineering array, has now been completed. It has allowed all of the sub-systems that will be used in the full instrument to be tested under field conditions. In this paper, the properties and performance of these sub-systems are described and their success illustrated with descriptions of some of the events recorded thus far.La lista completa de autores puede verse en el archivo asociado.Facultad de Ciencias Exactas2004-05-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf50-95http://sedici.unlp.edu.ar/handle/10915/78286enginfo:eu-repo/semantics/altIdentifier/issn/0168-9002info:eu-repo/semantics/altIdentifier/doi/10.1016/j.nima.2003.12.012info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/4.0/Creative Commons Attribution 4.0 International (CC BY 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T16:52:50Zoai:sedici.unlp.edu.ar:10915/78286Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 16:52:51.2SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Properties and performance of the prototype instrument for the Pierre Auger Observatory |
title |
Properties and performance of the prototype instrument for the Pierre Auger Observatory |
spellingShingle |
Properties and performance of the prototype instrument for the Pierre Auger Observatory Cillis, Analía Nilda Física Prototype instrument Pierre Auger Observatory Cosmic rays |
title_short |
Properties and performance of the prototype instrument for the Pierre Auger Observatory |
title_full |
Properties and performance of the prototype instrument for the Pierre Auger Observatory |
title_fullStr |
Properties and performance of the prototype instrument for the Pierre Auger Observatory |
title_full_unstemmed |
Properties and performance of the prototype instrument for the Pierre Auger Observatory |
title_sort |
Properties and performance of the prototype instrument for the Pierre Auger Observatory |
dc.creator.none.fl_str_mv |
Cillis, Analía Nilda Dova, María Teresa Epele, Luis Nicolás Grunfeld, Christian Martín Manceñido, Mónica E. Mariazzi, Analisa Gabriela Martínez, Nora Sciutto, Sergio Juan Veiga, Alejandro Luis The Pierre Auger Collaboration |
author |
Cillis, Analía Nilda |
author_facet |
Cillis, Analía Nilda Dova, María Teresa Epele, Luis Nicolás Grunfeld, Christian Martín Manceñido, Mónica E. Mariazzi, Analisa Gabriela Martínez, Nora Sciutto, Sergio Juan Veiga, Alejandro Luis The Pierre Auger Collaboration |
author_role |
author |
author2 |
Dova, María Teresa Epele, Luis Nicolás Grunfeld, Christian Martín Manceñido, Mónica E. Mariazzi, Analisa Gabriela Martínez, Nora Sciutto, Sergio Juan Veiga, Alejandro Luis The Pierre Auger Collaboration |
author2_role |
author author author author author author author author author |
dc.subject.none.fl_str_mv |
Física Prototype instrument Pierre Auger Observatory Cosmic rays |
topic |
Física Prototype instrument Pierre Auger Observatory Cosmic rays |
dc.description.none.fl_txt_mv |
Construction of the first stage of the Pierre Auger Observatory has begun. The aim of the Observatory is to collect unprecedented information about cosmic rays above 10^18 eV. The first phase of the project, the construction and operation of a prototype system, known as the engineering array, has now been completed. It has allowed all of the sub-systems that will be used in the full instrument to be tested under field conditions. In this paper, the properties and performance of these sub-systems are described and their success illustrated with descriptions of some of the events recorded thus far. La lista completa de autores puede verse en el archivo asociado. Facultad de Ciencias Exactas |
description |
Construction of the first stage of the Pierre Auger Observatory has begun. The aim of the Observatory is to collect unprecedented information about cosmic rays above 10^18 eV. The first phase of the project, the construction and operation of a prototype system, known as the engineering array, has now been completed. It has allowed all of the sub-systems that will be used in the full instrument to be tested under field conditions. In this paper, the properties and performance of these sub-systems are described and their success illustrated with descriptions of some of the events recorded thus far. |
publishDate |
2004 |
dc.date.none.fl_str_mv |
2004-05-01 |
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/10915/78286 |
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http://sedici.unlp.edu.ar/handle/10915/78286 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
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info:eu-repo/semantics/altIdentifier/issn/0168-9002 info:eu-repo/semantics/altIdentifier/doi/10.1016/j.nima.2003.12.012 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/4.0/ Creative Commons Attribution 4.0 International (CC BY 4.0) |
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openAccess |
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http://creativecommons.org/licenses/by/4.0/ Creative Commons Attribution 4.0 International (CC BY 4.0) |
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application/pdf 50-95 |
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