The exposure of the hybrid detector of the Pierre Auger Observatory

The Pierre Auger Observatory is a detector for ultra-high energy cosmic rays. It consists of a surface array to measure secondary particles at ground level and a fluorescence detector to measure the development of air showers in the atmosphere above the array. The ‘‘hybrid” detection mode combines t...

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Autores principales:	Badagnani, Daniel Omar, Dova, María Teresa, Gómez Albarracín, Flavia Alejandra, Hansen, Patricia María, Mariazzi, Analisa Gabriela, Moreno, Juan Cruz, Sciutto, Sergio Juan, Tarutina, Tatiana, Wahlberg, Hernán Pablo, The Pierre Auger Collaboration
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2010
Materias:	Ciencias Exactas Física Cascada atmosférica extensa Radiación cósmica Pierre Auger Observatory Fluorescencia
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/80654
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

id	I19-R120-10915-80654
record_format	dspace
institution	Universidad Nacional de La Plata
institution_str	I-19
repository_str	R-120
collection	SEDICI (UNLP)
language	Inglés
topic	Ciencias Exactas Física Cascada atmosférica extensa Radiación cósmica Pierre Auger Observatory Fluorescencia
spellingShingle	Ciencias Exactas Física Cascada atmosférica extensa Radiación cósmica Pierre Auger Observatory Fluorescencia Badagnani, Daniel Omar Dova, María Teresa Gómez Albarracín, Flavia Alejandra Hansen, Patricia María Mariazzi, Analisa Gabriela Moreno, Juan Cruz Sciutto, Sergio Juan Tarutina, Tatiana Wahlberg, Hernán Pablo The Pierre Auger Collaboration The exposure of the hybrid detector of the Pierre Auger Observatory
topic_facet	Ciencias Exactas Física Cascada atmosférica extensa Radiación cósmica Pierre Auger Observatory Fluorescencia
description	The Pierre Auger Observatory is a detector for ultra-high energy cosmic rays. It consists of a surface array to measure secondary particles at ground level and a fluorescence detector to measure the development of air showers in the atmosphere above the array. The ‘‘hybrid” detection mode combines the information from the two subsystems. We describe the determination of the hybrid exposure for events observed by the fluorescence telescopes in coincidence with at least one water-Cherenkov detector of the surface array. A detailed knowledge of the time dependence of the detection operations is crucial for an accurate evaluation of the exposure. We discuss the relevance of monitoring data collected during operations, such as the status of the fluorescence detector, background light and atmospheric conditions, that are used in both simulation and reconstruction.
format	Articulo Articulo
author	Badagnani, Daniel Omar Dova, María Teresa Gómez Albarracín, Flavia Alejandra Hansen, Patricia María Mariazzi, Analisa Gabriela Moreno, Juan Cruz Sciutto, Sergio Juan Tarutina, Tatiana Wahlberg, Hernán Pablo The Pierre Auger Collaboration
author_facet	Badagnani, Daniel Omar Dova, María Teresa Gómez Albarracín, Flavia Alejandra Hansen, Patricia María Mariazzi, Analisa Gabriela Moreno, Juan Cruz Sciutto, Sergio Juan Tarutina, Tatiana Wahlberg, Hernán Pablo The Pierre Auger Collaboration
author_sort	Badagnani, Daniel Omar
title	The exposure of the hybrid detector of the Pierre Auger Observatory
title_short	The exposure of the hybrid detector of the Pierre Auger Observatory
title_full	The exposure of the hybrid detector of the Pierre Auger Observatory
title_fullStr	The exposure of the hybrid detector of the Pierre Auger Observatory
title_full_unstemmed	The exposure of the hybrid detector of the Pierre Auger Observatory
title_sort	exposure of the hybrid detector of the pierre auger observatory
publishDate	2010
url	http://sedici.unlp.edu.ar/handle/10915/80654
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The exposure of the hybrid detector of the Pierre Auger Observatory

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