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The exposure of the hybrid detector of the Pierre Auger Observatory.

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dc.contributor.authorArganda, E.
dc.contributor.authorArqueros Martínez, Fernando
dc.contributor.authorBlanco Ramos, Francisco
dc.contributor.authorGarcía Pinto, Diego
dc.contributor.authorOrtiz Ramis, Montserrat
dc.contributor.authorRosado Vélez, Jaime
dc.contributor.authorVázquez Peñas, José Ramón
dc.date.accessioned2023-06-20T04:17:21Z
dc.date.available2023-06-20T04:17:21Z
dc.date.issued2011-01
dc.description© 2010 Elsevier B.V. Autoría conjunta: Pierre Auger Collaboration. Artículo firmado por más de 10 autores. We are very grateful to the following agencies and organizations for financial support: Comision Nacional de Energia Atomica, Fundacion Antorchas, Gobierno De La Provincia de Mendoza, Municipalidad de Malargue, NDM Holdings and Valle Las Lenas, in gratitude for their continuing cooperation over land access, Argentina; the Australian Research Council; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq), Financiadora de Estudos e Projetos (FINEP), Fundacao de Amparo a Pesquisa do Estado de Rio de Janeiro (FAPERJ), Fundacao de Amparo Pesquisa do Estado de Sao Paulo (FAPESP), Ministerio de Ciencia e Tecnologia (MCT), Brazil; AVCR AV0Z10100502 and AV0Z10100522, GAAV KJB300100801 and KJB100100904, MSMT-CR LA08016, LC527, 1M06002, and MSM0021620859, Czech Republic; Centre de Calcul IN2P3/CNRS, Centre National de la Recherche Scientifique (CNRS), Conseil Regional Ile-de-France, Departement Physique Nucleaire et Corpusculaire (PNC-IN2P3/CNRS), Departement Sciences de l'Univers (SDU-INSU/CNRS), France; Bundesministerium fur Bildung und Forschung (BMBF), Deutsche Forschungsgemeinschaft (DFG), Finanzministerium Baden-Wurttemberg, Helmholtz-Gemeinschaft Deutscher Forschungszentren (HGF), Ministerium fur Wissenschaft und Forschung, Nordrhein-Westfalen, Ministerium fur Wissenschaft, Forschung und Kunst, Baden-Wurttemberg, Germany; Istituto Nazionale di Fisica Nucleare (INFN), Istituto Nazionale di Astrofisica (INAF), Ministerodell'Istruzione, dell'Universita e della Ricerca(MIUR), Italy; Consejo Nacional de Ciencia y Tecnologia (CONACYT), Mexico; Ministerie van Onderwijs, Cultuur en Wetenschap, Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO), Stichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands; Ministry of Science and Higher Education, Grant Nos. 1 P03 D 014 30 and N N202 207238, Poland; Fundacao para a Ciencia e a Tecnologia, Portugal; Ministry for Higher Education, Science, and Technology, Slovenian Research Agency, Slovenia; Comunidad de Madrid, Consejeria de Educacion de la Comunidad de Castilla La Mancha, FEDER funds, Ministerio de Ciencia e Innovacion and Consolider-Ingenio 2010 (CPAN), Generalitat Valenciana, Junta de Andalucia, Xunta de Galicia, Spain; Science and Technology Facilities Council, United Kingdom; Department of Energy, Contract Nos. DE-AC02-07CH11359, DE-FR02-04ER41300, National Science Foundation, Grant No. 0450696, The Grainger Foundation USA; ALFA-EC/HELEN, European Union 6th Framework Program, Grant No. MEIF-CT-2005-025057, European Union 7th Framework Program, Grant No. PIEF-GA-2008-220240, and UNESCO.
dc.description.abstractThe 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. (C) 2010 Elsevier B.V. All rights reserved.
dc.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipAVCR, Czech Republic
dc.description.sponsorshipGAAV, Czech Republic
dc.description.sponsorshipMSMT-CR, Czech Republic
dc.description.sponsorshipCentre de Calcul
dc.description.sponsorshipCentre National de la Recherche Scientifique (CNRS)
dc.description.sponsorshipConseil Regional Ile-de-France
dc.description.sponsorshipDepartement Physique Nucleaire et Corpusculaire (PNC-IN2P3/CNRS)
dc.description.sponsorshipDepartement Sciences de l'Univers (SDU-INSU/CNRS), France
dc.description.sponsorshipBundesministerium fur Bildung und Forschung (BMBF)
dc.description.sponsorshipDeutsche Forschungsgemeinschaft (DFG)
dc.description.sponsorshipFinanzministerium Baden-Wurttemberg
dc.description.sponsorshipHelmholtz-Gemeinschaft Deutscher Forschungszentren (HGF)
dc.description.sponsorshipMinisterium fur Wissenschaft und Forschung Nordrhein-Westfalen
dc.description.sponsorshipMinisterium fur Wissenschaft, Forschung und Kunst, Baden-Wurttemberg, Germany
dc.description.sponsorshipIstituto Nazionale di Fisica Nucleare (INFN)
dc.description.sponsorshipMinisterodell'Istruzione, dell'Universita e della Ricerca(MIUR), Italy
dc.description.sponsorshipMinisterie van Onderwijs, Cultuur en Wetenschap, Netherlands
dc.description.sponsorshipNederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)
dc.description.sponsorshipStichting voor Fundamenteel Onderzoek der Materie (FOM), Netherlands
dc.description.sponsorshipFundacao para a Ciencia e a Tecnologia, Portugal
dc.description.sponsorshipMinistry of Science and Higher Education, Poland
dc.description.sponsorshipMinistry for Higher Education, Science, and Technology
dc.description.sponsorshipSlovenian Research Agency, Slovenia
dc.description.sponsorshipComunidad de Madrid
dc.description.sponsorshipConsejeria de Educacion de la Comunidad de Castilla La Mancha
dc.description.sponsorshipMinisterio de Ciencia e Innovacion and Consolider-Ingenio (CPAN), Spain
dc.description.sponsorshipFEDER funds, Spain
dc.description.sponsorshipGeneralitat Valenciana
dc.description.sponsorshipJunta de Andalucia
dc.description.sponsorshipXunta de Galicia, Spain
dc.description.sponsorshipScience and Technology Facilities Council, United Kingdom
dc.description.sponsorshipALFA-EC/HELEN
dc.description.sponsorshipEuropean Union 6th Framework Program
dc.description.sponsorshipEuropean Union 7th Framework Program
dc.description.sponsorshipUNESCO
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/39152
dc.identifier.doi10.1016/j.astropartphys.2010.10.001
dc.identifier.issn0927-6505
dc.identifier.officialurlhttp://dx.doi.org/10.1016/j.astropartphys.2010.10.001
dc.identifier.relatedurlhttp://www.sciencedirect.com/
dc.identifier.relatedurlhttp://arxiv.org/abs/1010.6162
dc.identifier.urihttps://hdl.handle.net/20.500.14352/45132
dc.issue.number6
dc.journal.titleAstroparticle physics
dc.language.isoeng
dc.page.final381
dc.page.initial368
dc.publisherElsevier Science BV
dc.relation.projectIDAUGERCRSOURCE (220240)
dc.relation.projectIDAV0Z10100502
dc.relation.projectIDAV0Z10100522
dc.relation.projectIDKJB300100801
dc.relation.projectIDKJB100100904
dc.relation.projectIDLA08016
dc.relation.projectIDLC527
dc.relation.projectID1M06002
dc.relation.projectIDMSM0021620859
dc.relation.projectIDIN2P3/CNRS
dc.relation.projectID1 P03 D 014 30
dc.relation.projectIDN N202 207238
dc.relation.projectIDMEIF-CT-2005-0250 P
dc.rights.accessRightsopen access
dc.subject.cdu539.1
dc.subject.keywordFluorescence detector
dc.subject.keywordEnergy spectrum
dc.subject.keywordSimulation
dc.subject.keywordShowers
dc.subject.keywordSystem.
dc.subject.ucmFísica nuclear
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleThe exposure of the hybrid detector of the Pierre Auger Observatory.
dc.typejournal article
dc.volume.number34
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