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dc.contributor.authorAlbert, A.
dc.contributor.authorDíaz García, Antonio Francisco 
dc.contributor.authorLópez Coto, Daniel 
dc.contributor.authorNavas Concha, Sergio 
dc.contributor.authorAntares Collaboration
dc.date.accessioned2021-06-18T10:56:21Z
dc.date.available2021-06-18T10:56:21Z
dc.date.issued2021-03-19
dc.identifier.citationA. Albert... [et al.]. Measurement of the atmospheric νe and νμ energy spectra with the ANTARES neutrino telescope, Physics Letters B, Volume 816, 2021, 136228, ISSN 0370-2693, [https://doi.org/10.1016/j.physletb.2021.136228]es_ES
dc.identifier.urihttp://hdl.handle.net/10481/69278
dc.descriptionThe authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l'Energie Atomique et aux Energies Alternatives(CEA), Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), Labex UnivEarthS(ANR-10-LABX-0023 and ANR-18-IDEX-0001), Region Ile-de-France (DIM-ACAV), Region Alsace (contrat CPER), Region Provence-AlpesCote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur Bildung und Forschung (BMBF), Germany; Instituto Nazionale di Fisica Nucleare(INFN), Italy; Nederlandse Organisatie voor Wetenschappelijk Onderzoek(NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; Executive Unit for Financing Higher Education, Research, Development and Innovation (UEFISCDI), Romania; Ministerio de Ciencia e Innovacion (MCI) and Agencia Estatal de Investigacion: Programa Estatal de Generacion de Conocimiento (refs. PGC2018096663-B-C41, -A-C42, -B-C43, -B-C44) (MCI/FEDER), Severo Ochoa Centre of Excellence and MultiDark Consolider, Junta de Andalucia (ref. SOMM17/6104/UGR and A-FQM-053-UGR18), Generalitat Valenciana: Grisolia (ref. GRISOLIA/2018/119) and GenT (ref. CIDEGENT/2018/034) programs, Spain; Ministry of Higher Education, Scientific Research and Professional Training, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities. The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l'Energie Atomique et aux Energies Alternatives(CEA), Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), Labex UnivEarthS(ANR-10-LABX-0023 and ANR-18-IDEX-0001), Region Ile-de-France (DIM-ACAV), Region Alsace (contrat CPER), Region Provence-AlpesCote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur Bildung und Forschung (BMBF), Germany; Instituto Nazionale di Fisica Nucleare(INFN), Italy; Nederlandse Organisatie voor Wetenschappelijk Onderzoek(NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; Executive Unit for Financing Higher Education, Research, Development and Innovation (UEFISCDI), Romania; Ministerio de Ciencia e Innovacion (MCI) and Agencia Estatal de Investigacion: Programa Estatal de Generacion de Conocimiento (refs. PGC2018096663-B-C41, -A-C42, -B-C43, -B-C44) (MCI/FEDER), Severo Ochoa Centre of Excellence and MultiDark Consolider, Junta de Andalucia (ref. SOMM17/6104/UGR and A-FQM-053-UGR18), Generalitat Valenciana: Grisolia (ref. GRISOLIA/2018/119) and GenT (ref. CIDEGENT/2018/034) programs, Spain; Ministry of Higher Education, Scientific Research and Professional Training, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities.es_ES
dc.description.abstractThis letter presents a combined measurement of the energy spectra of atmospheric nu(e) and nu(mu) in the energy range between similar to 100 GeV and similar to 50 TeV with the ANTARES neutrino telescope. The analysis uses 3012 days of detector livetime in the period 2007-2017, and selects 1016 neutrinos interacting in (or close to) the instrumented volume of the detector, yielding shower-like events (mainly from nu(e) + (nu) over bar (e) charged current plus all neutrino neutral current interactions) and starting track events (mainly from nu(mu) + (nu) over bar (mu) charged current interactions). The contamination by atmospheric muons in the final sample is suppressed at the level of a few per mill by different steps in the selection analysis, including a Boosted Decision Tree classifier. The distribution of reconstructed events is unfolded in terms of electron and muon neutrino fluxes. The derived energy spectra are compared with previous measurements that, above 100 GeV, are limited to experiments in polar ice and, for nu(mu), to Super-Kamiokande.es_ES
dc.description.sponsorshipCentre National de la Recherche Scientifique (CNRS)es_ES
dc.description.sponsorshipFrench Atomic Energy Commissiones_ES
dc.description.sponsorshipCommission Europeenne (FEDER fund)es_ES
dc.description.sponsorshipInstitut Universitaire de France (IUF)es_ES
dc.description.sponsorshipLabex UnivEarthS ANR-10-LABX-0023 ANR-18-IDEX-0001es_ES
dc.description.sponsorshipRegion Ile-de-Francees_ES
dc.description.sponsorshipRegion Grand-Estes_ES
dc.description.sponsorshipRegion Provence-Alpes-Cote d'Azures_ES
dc.description.sponsorshipRegion Provence-Alpes-Cote d'Azures_ES
dc.description.sponsorshipFederal Ministry of Education & Research (BMBF)es_ES
dc.description.sponsorshipInstituto Nazionale di Fisica Nucleare(INFN), Italyes_ES
dc.description.sponsorshipNetherlands Organization for Scientific Research (NWO)es_ES
dc.description.sponsorshipNetherlands Governmentes_ES
dc.description.sponsorshipCouncil of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russiaes_ES
dc.description.sponsorshipConsiliul National al Cercetarii Stiintifice (CNCS)es_ES
dc.description.sponsorshipUnitatea Executiva pentru Finantarea Invatamantului Superior, a Cercetarii, Dezvoltarii si Inovarii (UEFISCDI)es_ES
dc.description.sponsorshipSpanish Government PGC2018096663-B-C41 PGC2018096663-A-C42 PGC2018096663-B-C43 PGC2018096663-B-C44es_ES
dc.description.sponsorshipSevero Ochoa Centre of Excellence and MultiDark Consolideres_ES
dc.description.sponsorshipJunta de Andalucia SOMM17/6104/UGR A-FQM-053-UGR18es_ES
dc.description.sponsorshipGeneralitat Valenciana: Grisolia program, Spain GRISOLIA/2018/119es_ES
dc.description.sponsorshipGeneralitat Valenciana: GenT program, Spain CIDEGENT/2018/034es_ES
dc.description.sponsorshipMinistry of Higher Education, Scientific Research and Professional Training, Moroccoes_ES
dc.description.sponsorshipAgencia Estatal de Investigacion PGC2018096663-B-C41 PGC2018096663-A-C42 PGC2018096663-B-C43 PGC2018096663-B-C44es_ES
dc.description.sponsorshipCommission Europeenne (Marie Curie Program)es_ES
dc.language.isoenges_ES
dc.publisherElsevieres_ES
dc.rightsAtribución 3.0 España*
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/es/*
dc.subjectNeutrino telescopees_ES
dc.subjectAtmospheric neutrinoses_ES
dc.subjectANTARESes_ES
dc.titleMeasurement of the atmospheric νe and νμ energy spectra with the ANTARES neutrino telescopees_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES
dc.identifier.doi10.1016/j.physletb.2021.136228
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersiones_ES


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