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Record W2845504537 · doi:10.1126/science.aat1378

Multimessenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A

2018· article· en· W2845504537 on OpenAlexfundno aff

Bibliographic record

VenueScience · 2018
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsnot available
FundersLos Alamos National LaboratoryInstitute for Global Prominent Research, Chiba UniversityInstitut National de Physique Nucléaire et de Physique des ParticulesDeutsches Elektronen-SynchrotronEconomic and Social Research CouncilCenter for Cosmology and Astroparticle Physics, Ohio State UniversityMarsden FundInstituto de Astrofísica de CanariasHelmholtz Alliance for Astroparticle PhysicsIstituto Nazionale di Fisica NucleareUniversity of NamibiaNational Commission on Research, Science and TechnologyRWTH Aachen UniversityIstituto Nazionale di AstrofisicaHigh Energy Accelerator Research OrganizationHrvatska Zaklada za ZnanostOffice of ScienceNarodowym Centrum NaukiCollege of Engineering, Michigan State UniversityKnut och Alice Wallenbergs StiftelseGordon and Betty Moore FoundationPennsylvania State UniversityAgenzia Spaziale ItalianaFonds De La Recherche Scientifique - FNRSConselho Nacional de Desenvolvimento Científico e TecnológicoDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoConsejo Nacional de Ciencia y TecnologíaFonds Wetenschappelijk OnderzoekCentre National d’Etudes SpatialesBundesministerium für Bildung, Wissenschaft und ForschungDeutsche ForschungsgemeinschaftChinese Academy of SciencesNatural Sciences and Engineering Research Council of CanadaMinistry of Education, Culture, Sports, Science and TechnologyBundesministerium für Bildung und ForschungUniversiteit van AmsterdamVetenskapsrådetOhio State UniversityNational Research Foundation of KoreaNational Natural Science Foundation of ChinaSmithsonian InstitutionFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroU.S. Department of EnergyUniversity of Wisconsin-MadisonEuropean CommissionNational Radio Astronomy ObservatoryAustralian Research CouncilWestern Canada Research GridLaboratory Directed Research and DevelopmentMinistério da Ciência, Tecnologia, Inovações e ComunicaçõesMarquette UniversityChinese Academy of Sciences South America Center for AstronomyScience and Technology Facilities CouncilSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungBenemérita Universidad Autónoma de PueblaNational Astronomical Observatory of JapanEGI FederationJapan Aerospace Exploration AgencyJapan Society for the Promotion of ScienceVillum FondenAlexander von Humboldt-StiftungUniversity of PennsylvaniaAustrian Science FundNational Research CentreAssociated UniversitiesEuropean Regional Development FundCentre National de la Recherche ScientifiqueMax-Planck-GesellschaftUniversity of LeicesterNational Research FoundationPolarforskningssekretariatetDanmarks GrundforskningsfondCommissariat à l'Énergie Atomique et aux Énergies AlternativesNational Aeronautics and Space AdministrationOffice of Polar ProgramsMichigan State UniversityCompute CanadaChiba UniversityLiverpool John Moores UniversityBelgian Federal Science Policy OfficeNational Science Foundation
KeywordsBlazarNeutrinoSupernovaCosmic rayFlux (metallurgy)COSMIC cancer databaseCoincidence

Abstract

fetched live from OpenAlex

Previous detections of individual astrophysical sources of neutrinos are limited to the Sun and the supernova 1987A, whereas the origins of the diffuse flux of high-energy cosmic neutrinos remain unidentified. On 22 September 2017, we detected a high-energy neutrino, IceCube-170922A, with an energy of ~290 tera-electron volts. Its arrival direction was consistent with the location of a known γ-ray blazar, TXS 0506+056, observed to be in a flaring state. An extensive multiwavelength campaign followed, ranging from radio frequencies to γ-rays. These observations characterize the variability and energetics of the blazar and include the detection of TXS 0506+056 in very-high-energy γ-rays. This observation of a neutrino in spatial coincidence with a γ-ray-emitting blazar during an active phase suggests that blazars may be a source of high-energy neutrinos.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.007
Threshold uncertainty score0.013

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0010.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.012
GPT teacher head0.221
Teacher spread0.209 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations1,136
Published2018
Admission routes1
Has abstractyes

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