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

Kanata Swift/NuSTAR ddc:520 Astronomical Sciences Blazar blazar: emission 7. Clean energy Multidisciplinary, Blazar, Neutrino High Energy Physics - Experiment neutrino High Energy Physics - Experiment (hep-ex) ASAS-SN MISSION High Energy Astrophysical Phenomena (astro-ph.HE) Multidisciplinary ORIGIN Particle and High Energy Physics 001 Nuclear and Plasma Physics 520 Multidisciplinary Sciences gamma ray: emission H.E.S.S Physical Sciences Science & Technology - Other Topics VERITAS Kapteyn Astrophysics - High Energy Astrophysical Phenomena ACTIVE GALACTIC NUCLEI TELESCOPE General Science & Technology FOS: Physical sciences IceCube Collaboration 530 jet: relativistic AGILE Subaru Neutrino Kiso supernova SPECTROGRAPH neutrino event IceCube-170922A ; gamma-ray blazar TXS 0506+056 quasar Science & Technology ta115 INTEGRAL background Institut für Physik und Astronomie High energy neutrino Liverpool Telescope PERFORMANCE VLA/17B-403 teams MAGIC CRAB-NEBULA flux messenger gamma ray: VHE 13. Climate action Fermi-LAT [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph] [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] HAWC H.E.S.S.
DOI: 10.1126/science.aat1378 Publication Date: 2018-07-12T15:05:24Z
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ABSTRACT
Neutrino emission from a flaring blazar Neutrinos interact only very weakly with matter, but giant detectors have succeeded in detecting small numbers of astrophysical neutrinos. Aside from a diffuse background, only two individual sources have been identified: the Sun and a nearby supernova in 1987. A multiteam collaboration detected a high-energy neutrino event whose arrival direction was consistent with a known blazar—a type of quasar with a relativistic jet oriented directly along our line of sight. The blazar, TXS 0506+056, was found to be undergoing a gamma-ray flare, prompting an extensive multiwavelength campaign. Motivated by this discovery, the IceCube collaboration examined lower-energy neutrinos detected over the previous several years, finding an excess emission at the location of the blazar. Thus, blazars are a source of astrophysical neutrinos. Science , this issue p. 147 , p. eaat1378
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