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Tyler J, Vassiliev V, Wakely S, Weinstein A, Wells R, Wilcox P, Wilhelm A, Williams D, Zitzer B, Tetarenko A, Kimball A, Miller-Jones J, Sivakoff G. Multimessenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A. Science 2018; 361:science.aat1378. [DOI: 10.1126/science.aat1378] [Citation(s) in RCA: 451] [Impact Index Per Article: 64.4] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/09/2018] [Accepted: 06/08/2018] [Indexed: 11/02/2022]
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 ~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.
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