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Very high-energy gamma-ray follow-up program using neutrino triggers from IceCube

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dc.contributor.authorBarrio Uña, Juan Abel
dc.contributor.authorBonnefoy, Simon Francois Albert
dc.contributor.authorContreras González, José Luis
dc.contributor.authorDomínguez, A.
dc.contributor.authorFidalgo, D.
dc.contributor.authorFonseca González, María Victoria
dc.contributor.authorLópez, M.
dc.contributor.authorNievas Rosillo, Mireia
dc.date.accessioned2023-06-17T22:00:16Z
dc.date.available2023-06-17T22:00:16Z
dc.date.issued2016-11
dc.description© 2016 IOP Publishing Ltd and Sissa Medialab srl Artículo firmado por más de 10 autores We acknowledge the support from the following agencies: U.S. National Science Foundation-Office of Polar Programs, U.S. National Science Foundation-Physics Division, University of Wisconsin Alumni Research Foundation, the Grid Laboratory Of Wisconsin (GLOW) grid infrastructure at the University of Wisconsin - Madison, the Open Science Grid (OSG) grid infrastructure; U.S. Department of Energy, and National Energy Research Scientific Computing Center, the Louisiana Optical Network Initiative (LONI) grid computing resources; Natural Sciences and Engineering Research Council of Canada, WestGrid and Compute/Calcul Canada; Swedish Research Council, Swedish Polar Research Secretariat, Swedish National Infrastructure for Computing (SNIC), and Knut and Alice Wallenberg Foundation, Sweden; German Ministry for Education and Research (BMBF), Deutsche Forschungsgemeinschaft (DFG), Helmholtz Alliance for Astroparticle Physics (HAP), Research Department of Plasmas with Complex Interactions (Bochum), Germany; Fund for Scientific Research (FNRS-FWO), FWO Odysseus programme, Flanders Institute to encourage scientific and technological research in industry (IWT), Belgian Federal Science Policy Office (Belspo); University of Oxford, United Kingdom; Marsden Fund, NewZealand; Australian Research Council; Japan Society for Promotion of Science (JSPS); the Swiss National Science Foundation (SNSF), Switzerland; National Research Foundation of Korea (NRF); Villum Fonden, Danish National Research Foundation (DNRF), Denmark.; The VERITAS Collaboration acknowledges the support of the U.S. Department of Energy Office of Science, the U.S. National Science Foundation and the Smithsonian Institution, and NSERC in Canada. We also acknowledge the excellent work of the technical support staff at the Fred Lawrence Whipple Observatory and at the collaborating institutions in the construction and operation of the instrument.; The MAGIC collaboration would like to thank the Instituto de Astrofisica de Canarias for the excellent working conditions at the Observatorio del Roque de los Muchachos in La Palma. The financial support of the German BMBF and MPG, the Italian INFN and INAF, the Swiss National Fund SNF, the he ERDF under the Spanish MINECO (FPA2015-69818-P, FPA2012-36668, FPA2015-68278-P, FPA2015-69210-C6-2-R, FPA2015-69210-C6-4-R, FPA2015-69210-C6-6-R, AYA2013-47447-C3-1-P, AYA2015-71042-P, ESP2015-71662-C2-2-P, CSD2009-00064), and the Japanese JSPS and MEXT is gratefully acknowledged. This work was also supported by the Spanish Centro de Excelencia "Severo Ochoa" SEV-2012-0234 and SEV-2015-0548, and Unidad de Excelencia "Maria de Maeztu" MDM-2014-0369, by grant 268740 of the Academy of Finland, by the Croatian Science Foundation (HrZZ) Project 09/176 and the University of Rijeka Project 13.12.1.3.02, by the DFG Collaborative Research Centers SFB823/C4 and SFB876/C3, and by the Polish MNiSzW grant 745/N-HESS-MAGIC/2010/0.
dc.description.abstractWe describe and report the status of a neutrino-triggered program in IceCube that generates real-time alerts for gamma-ray follow-up observations by atmospheric-Cherenkov telescopes (MAGIC and VERITAS). While IceCube is capable of monitoring the whole sky continuously, high-energy gamma-ray telescopes have restricted fields of view and in general are unlikely to be observing a potential neutrino-flaring source at the time such neutrinos are recorded. The use of neutrino-triggered alerts thus aims at increasing the availability of simultaneous multi-messenger data during potential neutrino flaring activity, which can increase the discovery potential and constrain the phenomenological interpretation of the high-energy emission of selected source classes (e. g. blazars). The requirements of a fast and stable online analysis of potential neutrino signals and its operation are presented, along with first results of the program operating between 14 March 2012 and 31 December 2015.
dc.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipMinisterio de Economía y Competitividad (MINECO)
dc.description.sponsorshipSwedish Research Council
dc.description.sponsorshipSwedish Polar Research Secretariat
dc.description.sponsorshipSwedish National Infrastructure for Computing (SNIC)
dc.description.sponsorshipKnut and Alice Wallenberg Foundation, Sweden
dc.description.sponsorshipGerman Ministry for Education and Research (BMBF)
dc.description.sponsorshipDeutsche Forschungsgemeinschaft (DFG)
dc.description.sponsorshipHelmholtz Alliance for Astroparticle Physics (HAP)
dc.description.sponsorshipResearch Department of Plasmas with Complex Interactions (Bochum), Germany
dc.description.sponsorshipFund for Scientific Research (FNRS-FWO)
dc.description.sponsorshipFWO Odysseus programme
dc.description.sponsorshipFlanders Institute to encourage scientific and technological research in industry (IWT)
dc.description.sponsorshipBelgian Federal Science Policy Office (Belspo)
dc.description.sponsorshipUniversity of Oxford, United Kingdom
dc.description.sponsorshipSwiss National Science Foundation (SNSF), Switzerland
dc.description.sponsorshipVillum Fonden, Danish National Research Foundation (DNRF), Denmark
dc.description.sponsorshipGerman BMBF and MPG
dc.description.sponsorshipItalian INFN and INAF
dc.description.sponsorshipSpanish Centro de Excelencia "Severo Ochoa"
dc.description.sponsorshipUnidad de Excelencia "Maria de Maeztu"
dc.description.sponsorshipAcademy of Finland
dc.description.sponsorshipCroatian Science Foundation (HrZZ) Project
dc.description.sponsorshipUniversity of Rijeka Project
dc.description.sponsorshipDFG Collaborative Research Centers
dc.description.sponsorshipPolish MNiSzW
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/43818
dc.identifier.doi10.1088/1748-0221/11/11/P11009
dc.identifier.issn1748-0221
dc.identifier.officialurlhttp://dx.doi.org/10.1088/1748-0221/11/11/P11009
dc.identifier.relatedurlhttp://iopscience.iop.org
dc.identifier.urihttps://hdl.handle.net/20.500.14352/17915
dc.journal.titleJournal of instrumentation
dc.language.isoeng
dc.publisherIOP Publishing LTD
dc.relation.projectIDFPA2015-69818-P
dc.relation.projectIDFPA2012-36668
dc.relation.projectIDFPA2015-68278-P
dc.relation.projectIDFPA2015-69210-C6-2-R
dc.relation.projectIDFPA2015-69210-C6-4-R
dc.relation.projectIDFPA2015-69210-C6-6-R
dc.relation.projectIDAYA2013-47447-C3-1-P
dc.relation.projectIDAYA2015-71042-P
dc.relation.projectIDESP2015-71662-C2-2-P
dc.relation.projectIDCSD2009-00064
dc.relation.projectIDSEV-2012-0234
dc.relation.projectIDSEV-2015-0548
dc.relation.projectIDMDM-2014-0369
dc.relation.projectID268740
dc.relation.projectID09/176
dc.relation.projectID13.12.1.3.02
dc.relation.projectIDSFB823/C4
dc.relation.projectIDSFB876/C3
dc.relation.projectID745/N-HESS-MAGIC/2010/0
dc.rights.accessRightsopen access
dc.subject.cdu539.1
dc.subject.keywordBL Lacertae objects
dc.subject.keywordActive galactic nuclei
dc.subject.keywordXmm Newton
dc.subject.keywordMultiwavelength observations
dc.subject.keywordCorrelated variability
dc.subject.keywordLac objects
dc.subject.keywordBlazars
dc.subject.keywordMarkarian 421
dc.subject.keywordTelescope
dc.subject.keywordEmission
dc.subject.ucmFísica nuclear
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleVery high-energy gamma-ray follow-up program using neutrino triggers from IceCube
dc.typejournal article
dc.volume.number11
dspace.entity.typePublication
relation.isAuthorOfPublication11e5fd8b-1a86-4f8d-85c6-135541232be4
relation.isAuthorOfPublication6a14529e-a65e-4709-9bc1-61f9429841c1
relation.isAuthorOfPublication9f2c0e34-0edd-497a-bbd0-fbd9d348e85c
relation.isAuthorOfPublication355179c2-4111-4313-8c52-8bfc0775c2b3
relation.isAuthorOfPublication.latestForDiscovery11e5fd8b-1a86-4f8d-85c6-135541232be4

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