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

  • Icecube Collaboration
  • , Fermi-LAT collaboration
  • , MAGIC Collaboration
  • , AGILE
  • , ASAS-SN
  • , HAWC
  • , H.E.S.S.
  • , INTEGRAL
  • , Kanata, Kiso, and Subaru observing teams
  • , Kapteyn
  • , Liverpool telescope
  • , Swift/NuSTAR
  • , VERITAS
  • , VLA/17B-403 team
  • University of Canterbury
  • DESY
  • ULB Center for Diabetes Research
  • Niels Bohr Institutet
  • Oskar Klein Centre
  • University of Geneva
  • University of Erlangen-Nuremberg
  • Marquette University
  • Methodology Center at Penn State
  • Massachusetts Institute of Technology
  • RWTH Aachen University
  • South Dakota School of Mines and Technology
  • University of Alberta
  • University of California, Irvine
  • Johannes-Gutenberg University of Mainz
  • University of California Berkeley
  • Ohio State University
  • Ruhr-Universität Bochum
  • University of Wuppertal
  • University of Rochester
  • University of Maryland
  • University of Padova
  • Humboldt Universität zu Berlin
  • Univ. Kansas
  • Lawrence Berkeley National Laboratory
  • Technische Universität Dortmund
  • Uppsala University
  • University of Wisconsin-Madison
  • SNOLAB
  • University of Münster
  • Technical University Munich
  • Vrije Universiteit Brussel
  • Pennsylvania State University
  • Georgia Institute of Technology
  • Michigan State University
  • The Bartol Research Institute
  • Ghent University
  • Centro Universitario de Ciencias Biólogicas Y Agropecuarias, Centro de Estudios en Zoología, Universidad de Guadalajara
  • Sungkyunkwan University
  • Southern University and A&M College
  • University of Adelaide
  • University of Tokyo
  • Chiba University
  • Clark-Atlanta University
  • The University of Texas at Arlington
  • Stony Brook University
  • University of Alabama
  • Drexel University
  • University of Wisconsin-River Falls
  • Yale University
  • University of Alaska Anchorage
  • University of Oxford
  • University of California, Los Angeles
  • Hiroshima University
  • Clemson University
  • Max-Planck-Institut für Radioastronomie
  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
  • CEA Saclay
  • Istituto Nazionale di Fisica Nucleare, Sezione di Trieste
  • University of Trieste
  • Istituto Nazionale di Fisica Nucleare, Sezione di Padova
  • LSST Project Office
  • California State University Los Angeles
  • Dell'Universit e Del Politecnico di Bari
  • Istituto Nazionale di Fisica Nucleare, Sezione di Bari
  • Stanford University
  • Istituto Nazionale di Fisica Nucleare, Sezione di Torino
  • University of Turin
  • Université Montpellier 2
  • Laboratoire Leprince-Ringuet
  • University of Washington
  • NASA Goddard Space Flight Center
  • NASA Postdoctoral Program Fellow
  • INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica
  • INAF National Institute for Astrophysics
  • Agenzia Spaziale Italiana
  • Naval Research Laboratory
  • Istituto Nazionale di Fisica Nucleare, Sezione di Perugia
  • Stockholm University
  • Wallenberg Academy Fellow
  • INAF Istituto di Radioastronomia
  • University of Bologna
  • Università Telematica Pegaso
  • Complutense University
  • UMR 5797
  • Université Bordeaux
  • George Washington University
  • Konan University
  • Kyoto University
  • Tokai University
  • Tokushima University
  • Nova Southeastern University
  • University of Iceland
  • KTH Royal Institute of Technology
  • University of Wuerzburg
  • University of Amsterdam
  • University of Amsterdam
  • University of Udine
  • INFN Roma Tor Vergata
  • INFN–Roma Tor Vergata
  • INAF - Osservatorio Astronomico di Trieste
  • University and Research (MIUR)
  • University of Johannesburg
  • University of Innsbruck
  • UPMC Univ. Paris 06
  • Santa Cruz Institute for Particle Physics
  • University of Hong Kong
  • NYCB Real-Time Computing Inc.
  • Purdue University Calumet
  • Nagoya University
  • Max-Planck-Institut fur Physik
  • IRAP
  • Institut de Ciéncies de l’Espai (ICE-CSIC)
  • ICREA Catalan Institution for Research and Advanced Studies
  • INAF Osservatorio di Astrofisica e Scienza dello Spazio di Bologna
  • University of Perugia
  • Praxis Inc.
  • University of Nova Gorica
  • ETH Zürich
  • University of Rijeka
  • Faculty of Electrical Engineering, Mechanical Engineering and Naval Architecture, University of Split
  • The University of Osijek
  • Saha Institute of Nuclear Physics
  • Centro Brasileiro de Pesquisas Fisicas (CBPF/MCTI)
  • GTC Project
  • Universidad de la Laguna
  • University of Lodz
  • Campus UAB
  • University of Siena
  • U1038
  • Port d'Informació Científica (PIC)
  • University of Turku
  • University of Oulu
  • Autonomous University of Barcelona (UAB)
  • University of Barcelona
  • Instytut Fizyki Jadrowej PAN
  • Systems Glycobiology Research Group
  • Inst. for Nucl. Research and Nucl. Energy
  • University of Pisa
  • ASI Space Science Data Center (SSDC)
  • INAF–OAR
  • University of Rome "Tor Vergata"
  • Gran Sasso Science Institute
  • INFN–Pavia
  • University of Witwatersrand
  • INFN–Roma Sapienza
  • East Windsor RSD
  • Osservatorio Astronomico di Cagliari
  • INFN–Roma Tor Vergata
  • Osservatorio Astronomico di Brera
  • The Observatories of the Carnegie Institution for Science
  • Tsinghua University
  • Universidad Diego Portales
  • Millennium Institute of Astrophysics
  • Aarhus University
  • University of Utah
  • Los Alamos National Laboratory
  • UNAM
  • Universidad Autónoma de Chiapas
  • Universidad Michoacana de San Nicolás de Hidalgo
  • Óptica y Electrónica
  • Max-Planck-Institut fur Kernphysik
  • Benemérita Universidad Autónoma de Puebla
  • George Mason University
  • Michigan Technological University
  • NASA Marshall Space Flight Center
  • University of New Mexico
  • Universidad Politecnica de Pachuca
  • Instituto Politécnico Nacional
  • Cinvestav-IPN
  • Universidad Autónoma del Estado de Hidalgo
  • Instituto de Ciencias Nucleares de la UNAM
  • North-West University
  • Aix Marseille Université
  • University of Namibia
  • Linnaeus University, Växjö
  • Université PSL
  • Sorbonne Université
  • University of Warsaw
  • Université Paris Cité
  • University of Potsdam
  • Landessternwarte Heidelberg
  • Université Paris-Sud
  • University of Tübingen
  • Laboratoire Astrophysique de Grenoble
  • Uniwersytet Jagielloński
  • N. Copernicus Astronomical Center
  • University of Leicester
  • Heidelberg University
  • University of Adelaide
  • University of the Free State
  • University of Geneva
  • Max-Planck-Institut für Extraterrestrische Physik (MPE)
  • European Space Research and Technology Centre (ESTEC)
  • Graduate School of Science
  • Stanford University
  • National Institutes of Natural Sciences - National Astronomical Observatory of Japan
  • Ehime University
  • Tokyo Institute of Technology
  • Liverpool John Moores University
  • University of Maryland, College Park
  • Washington University in St. Louis
  • Harvard & Smithsonian
  • Columbia University
  • California Polytechnic State University, San Luis Obispo
  • University of Galway
  • Purdue University
  • Tsinghua University
  • McGill University
  • University of Minnesota
  • California State University, East Bay
  • University of Iowa
  • DePauw University
  • Iowa State University
  • Barnard College
  • University College Dublin
  • University of Chicago
  • South Campus
  • National Radio Astronomy Observatory Socorro
  • University of California, Santa Cruz

Research output: Contribution to a Journal (Peer & Non Peer) › Article › peer-review

1244 Citations (Scopus)

Abstract

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 e290 tera-electron volts. Its arrival direction was consistent with the location of a known g-ray blazar, TXS 0506+056, observed to be in a flaring state. An extensive multiwavelength campaign followed, ranging from radio frequencies to g-rays. These observations characterize the variability and energetics of the blazar and include the detection of TXS 0506+056 in very-high-energy g-rays. This observation of a neutrino in spatial coincidence with a g-ray-emitting blazar during an active phase suggests that blazars may be a source of high-energy neutrinos.

Original languageEnglish
Article numbereaat1378
JournalScience
Volume361
Issue number6398
DOIs
Publication statusPublished - 13 Jul 2018

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