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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
  • German Electron Synchrotron
  • Université libre de Bruxelles
  • University of Copenhagen
  • Oskar Klein Centre
  • University of Geneva
  • Friedrich-Alexander University Erlangen-Nürnberg
  • Klingler College of Arts and Sciences
  • Pennsylvania State University
  • Massachusetts Institute of Technology
  • RWTH Aachen University
  • South Dakota School of Mines & Technology
  • University of Alberta
  • University of California at Irvine
  • Johannes Gutenberg University Mainz
  • University of California at Berkeley
  • Ohio State University
  • Ruhr University Bochum
  • University of Wuppertal
  • University of Rochester
  • University of Maryland
  • University of Padua
  • Humboldt University of Berlin
  • University of Kansas
  • Lawrence Berkeley National Laboratory
  • TU Dortmund University
  • Uppsala University
  • University of Wisconsin-Madison
  • SNOLAB
  • University of Münster
  • Technical University of Munich
  • Vrije Universiteit Brussel
  • Georgia Institute of Technology
  • Michigan State University
  • University of Delaware
  • Ghent University
  • Universidad de Guadalajara
  • Sungkyunkwan University
  • Southern University and A&M College
  • University of Adelaide
  • The University of Tokyo
  • Chiba University
  • Clark Atlanta University
  • University of Texas at Arlington
  • Stony Brook University
  • Department of Physics and Astronomy
  • Drexel University
  • University of Wisconsin-River Falls
  • Yale University
  • University of Alaska Anchorage
  • University of Oxford
  • University of California at Los Angeles
  • Hiroshima University
  • Clemson University
  • Max Planck Institute for Radio Astronomy
  • National Institute for Nuclear Physics
  • CEA-IRFU/CNRS/Université Paris Diderot
  • University of Trieste
  • Large Synoptic Survey Telescope
  • California State University Los Angeles
  • Polytechnic University of Bari
  • Stanford University
  • University of Turin
  • Université Montpellier 2
  • Laboratoire Leprince-Ringuet
  • University of Washington
  • NASA Goddard Space Flight Center
  • NASA Postdoctoral Program Fellow
  • Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
  • National Institute for Astrophysics
  • Italian Space Agency
  • Naval Research Laboratory
  • Stockholm University
  • Wallenberg Academy Fellow
  • University of Bologna
  • Pegaso Telematic University
  • Complutense University
  • IN2P3 - Institut National de Physique Nucléaire et de Physique Des Particules
  • Centre d'Etudes Nucléaires Bordeaux-Gradingnan (CENBG)
  • George Washington University
  • Konan University
  • Kyoto University
  • Tokai University
  • Tokushima University
  • University of North Florida
  • University of Iceland
  • KTH Royal Institute of Technology
  • University of Würzburg
  • University of Amsterdam
  • University of Udine
  • INFN–Roma Tor Vergata
  • Osservatorio Astronomico di Trieste
  • University and Research (MIUR)
  • University of Innsbruck
  • Université Pierre et Marie Curie
  • University of California at Santa Cruz
  • The University of Hong Kong
  • NYCB Real-Time Computing Inc.
  • Purdue University Northwest
  • Nagoya University
  • Max Planck Institute for Physics (Werner Heisenberg Institute)
  • IRAP
  • Campus UAB
  • ICREA
  • University of Perugia
  • Praxis, Inc.
  • University of Nova Gorica
  • Swiss Federal Institute of Technology Zurich
  • University of Rijeka
  • University of Split
  • Josip Juraj Strossmayer University of Osijek
  • Saha Institute of Nuclear Physics
  • Centro Brasileiro de Pesquisas Físicas
  • Instituto de Astrofísica de Canarias
  • University of La Laguna
  • University of Łódź
  • Institute for High Energy Physics
  • University of Siena
  • Université Grenoble Alpes
  • Port d'Informació Científica (PIC)
  • University of Turku
  • University of Oulu
  • Autonomous University of Barcelona
  • University of Barcelona
  • Cracow
  • RIKEN
  • Bulgarian Academy of Sciences
  • University of Pisa
  • ASI - Space Science Data Center
  • INAF–OAR
  • University of Rome Tor Vergata
  • Gran Sasso Science Institute
  • INFN–Pavia
  • University of the Witwatersrand
  • INFN–Roma Sapienza
  • East Windsor RSD
  • INFN–Roma Tor Vergata
  • Osservatorio Astronomico di Brera
  • Carnegie Institution of Washington
  • Peking University
  • Universidad Diego Portales
  • Instituto Milenio de Astrofísica
  • Aarhus University
  • University of Utah
  • Los Alamos National Laboratory
  • Universidad Nacional Autónoma de México
  • Universidad Autonoma de Chiapas
  • Universidad Michoacana de San Nicolas de Hidalgo
  • Instituto Nacional de Astrofisica Optica y Electronica
  • Max Planck Institute for Nuclear Physics
  • Benemerita Universidad Autonoma de Puebla
  • George Mason University
  • Michigan Technological University
  • NASA Marshall Space Flight Center
  • University of New Mexico
  • Universidad Politecnica de Pachuca
  • Instituto Politécnico Nacional
  • Centro de Investigacion y de Estudios Avanzados del Instituto Politécnico Nacional
  • Universidad Autonoma del Estado de Hidalgo
  • North West University
  • Aix-Marseille Université
  • University of Namibia
  • Linnaeus University
  • PSL University
  • Sorbonne Université
  • University of Warsaw
  • Université de Paris
  • University of Potsdam
  • Heidelberg University 
  • Université Paris-Saclay
  • University of Tübingen
  • IPAG
  • Jagiellonian University in Kraków
  • Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences
  • University of Leicester
  • University of The Free State
  • Max Planck Institute for Extraterrestrial Physics
  • ESTEC
  • Kavli Institute for Particle Astrophysics and Cosmology
  • 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 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
  • University College Dublin
  • The University of Chicago
  • Munster Technological University
  • National Science Foundation

Research output: Contribution to journalArticlepeer-review

1225 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

ASJC Scopus subject areas

  • Multidisciplinary

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