Calibration of the underground muon detector of the Pierre Auger Observatory

dc.citation.titleJournal of Instrumentationes
dc.citation.volume16
dc.creatorThe Pierre Auger collaboration
dc.creatorFreire, M. M.
dc.creatorMicheletti, M. I.
dc.date.accessioned2022-04-12T17:36:31Z
dc.date.available2022-04-12T17:36:31Z
dc.date.issued2021-04-06
dc.descriptionTo obtain direct measurements of the muon content of extensive air showers with energy above 1016.5 eV, the Pierre Auger Observatory is currently being equipped with an underground muon detector (UMD), consisting of 219 10 m2-modules, each segmented into 64 scintillators coupled to silicon photomultipliers (SiPMs). Direct access to the shower muon content allows for the study of both of the composition of primary cosmic rays and of high-energy hadronic interactions in the forward direction. As the muon density can vary between tens of muons per m2 close to the intersection of the shower axis with the ground to much less than one per m2 when far away, the necessary broad dynamic range is achieved by the simultaneous implementation of two acquisition modes in the read-out electronics: the binary mode, tuned to count single muons, and the ADC mode, suited to measure a high number of them. In this work, we present the end-to-end calibration of the muon detector modules: first, the SiPMs are calibrated by means of the binary channel, and then, the ADC channel is calibrated using atmospheric muons, detected in parallel to the shower data acquisition. The laboratory and field measurements performed to develop the implementation of the full calibration chain of both binary and ADC channels are presented and discussed. The calibration procedure is reliable to work with the high amount of channels in the UMD, which will be operated continuously, in changing environmental conditions, for several years.es
dc.description.filFil: Freire, M. M. Universidad Nacional de Rosario. Facultad de Ciencias Bioquímicas y Farmacéuticas. Instituto de Física de Rosario (IFIR-CONICET); Argentina.es
dc.description.filFil: Micheletti, M. I. Universidad Nacional de Rosario. Facultad de Ciencias Bioquímicas y Farmacéuticas. Instituto de Física de Rosario (IFIR-CONICET); Argentina.es
dc.description.sponsorshipDirectorate for Mathematical and Physical Sciences (MPS): 0450696
dc.description.sponsorshipComisión Nacional de Energía Atómica
dc.description.sponsorshipAgencia Nacional de Promoción Científica y Tecnológica (ANPCyT)
dc.description.sponsorshipConsejo Nacional de Investigaciones Científicas y Técnicas (CONICET)
dc.description.sponsorshipThe Australian Research Council
dc.description.sponsorshipConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
dc.description.sponsorshipFinanciadora de Estudos e Projetos (FINEP)
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de Rio de Janeiro (FAPERJ)
dc.description.sponsorshipSão Paulo Research Foundation (FAPESP): 2019/10151-2, 2010/07359-6, 1999/05404-3
dc.description.sponsorshipMinistério da Ciência, Tecnologia, Inovações e Comunicações (MCTIC)
dc.description.sponsorshipCentre National de la Recherche Scientifique (CNRS)
dc.description.sponsorshipConseil Régional Ile-de-France
dc.description.sponsorshipDépartement Physique Nucléaire et Corpusculaire: PNC-IN2P3/CNRS
dc.description.sponsorshipDépartement Sciences de l´Univers: SDU-INSU/CNRS
dc.description.sponsorshipInstitut Lagrange de Paris (ILP): LABEX ANR-10-LABX-63
dc.description.sponsorshipInvestissements d´Avenir Programme: ANR-11-IDEX-0004-02
dc.description.sponsorshipBundesministerium für Bildung und Forschung (BMBF)
dc.description.sponsorshipDeutsche Forschungsgemeinschaft (DFG)
dc.description.sponsorshipFinanzministerium Baden-Württember
dc.description.sponsorshipHelmholtz Alliance for Astroparticle Physics (HAP)
dc.description.sponsorshipHelmholtz-Gemeinschaft Deutscher Forschungszentren (HGF)
dc.description.sponsorshipMinisterium für Innovation
dc.description.sponsorshipWissenschaft und Forschung des Landes Nordrhein-Westfalen
dc.description.sponsorshipMinisterium für Wissenschaft
dc.description.sponsorshipForschung und Kunst des Landes Baden-Württemberg
dc.description.sponsorshipIstituto Nazionale di Fisica Nucleare (INFN)
dc.description.sponsorshipIstituto Nazionale di Astrofisica (INAF)
dc.description.sponsorshipMinistero dell´ Iistruzione
dc.description.sponsorshipdell´ Universitá e della Ricerca (MIUR)
dc.description.sponsorshipCETEMPS Center of Excellence
dc.description.sponsorshipMinistero Degli Affari Esteri (MAE)
dc.description.sponsorshipConsejo Nacional de Ciencia y Tecnología (CONACYT)
dc.description.sponsorshipUniversidad Nacional Autónoma de México (UNAM)
dc.description.sponsorshipMinistry of Education, Culture and Science, Netherlands Organisation for Scientific Research (NWO)
dc.description.sponsorshipDutch national eMinfrastructure with the support of SURF Cooperative
dc.description.sponsorshipMinistry of Science and Higher Education: DIR/WK/2018/11
dc.description.sponsorshipNational Science Centre: 2013/08/MST9/00322, 2016/23/B/ST9/01635, HARMONIA 5-2013/10/M/ST9/00062, UMO-2016/22/M/ST9/00198
dc.description.sponsorshipPortuguese national funds and FEDER funds within Programa Operacional Factores de Competitividade through Fundação para a Ciência e a Tecnologia (COMPETE)
dc.description.sponsorshipRomanian Ministry of Education and Research
dc.description.sponsorshipSlovenian Research Agency: P1-0031, P1-0385, IO-0033, N1-0111
dc.description.sponsorshipMinisterio de Economía, Industria y Competitividad: FPA2017-85114-9, PID2019-104676GB-C32
dc.description.sponsorshipXunta de Galicia: ED431 2017/07
dc.description.sponsorshipJunta de Andalucía: SOMM17/6104/UGR, P18-FR-4314
dc.description.sponsorshipFeder Funds, RENATA Red Nacional Temática de Astropartículas: FPA2015-68783-REDT
dc.description.sponsorshipMaría de Maeztu Unit of Excellence: MDM-2016-0692
dc.description.sponsorshipDepartment of Energy: DE-AC02-07CH11359, DE-FR02-04ER41300, DE-FG02-99ER41107, DE-SC0011689
dc.description.sponsorshipNational Science Foundation: 0450696
dc.description.sponsorshipThe Grainger Foundation
dc.description.sponsorshipMarie-Curie-IRSES/EPLANET
dc.description.sponsorshipEuropean Particle Physics Latin American Network
dc.description.sponsorshipUnited Nations Educational, Scientific and Cultural Organization (UNESCO)
dc.formatapplication/pdf
dc.format.extent1-24es
dc.identifier.issn1938-1328es
dc.identifier.urihttp://hdl.handle.net/2133/23409
dc.language.isoenges
dc.publisherIOP Publishinges
dc.relation.publisherversionhttps://doi.org/10.1088/1748-0221/16/04/P04003
dc.relation.publisherversionhttps://iopscience.iop.org/article/10.1088/1748-0221/16/04/P04003
dc.rightsopenAccesses
dc.rights.holderThe Pierre Auger collaborationes
dc.rights.holderFreire, M. M.es
dc.rights.holderMicheletti, M. I.es
dc.rights.textAttribution 4.0 International (CC BY 4.0)es
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/*
dc.subjectParticle detectorses
dc.subjectDetector alignment and calibration methodses
dc.subjectPhoton detectors for uvLes
dc.subjectPerformance of high energy physics detectorses
dc.subjectVisible and ir photonses
dc.titleCalibration of the underground muon detector of the Pierre Auger Observatoryes
dc.typepublishedVersion
dc.typearticle
dc.typeartículo
dc.type.collectionarticulo
dc.type.versionpublishedVersion

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