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      A Search for Ultra-high-energy Neutrinos from TXS 0506+056 Using the Pierre Auger Observatory

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          Is Open Access

          Multi-messenger Observations of a Binary Neutron Star Merger

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

            (2018)
            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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              Detecting ντ oscillations at PeV energies

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                Author and article information

                Journal
                The Astrophysical Journal
                ApJ
                American Astronomical Society
                1538-4357
                October 01 2020
                October 16 2020
                : 902
                : 2
                : 105
                Article
                10.3847/1538-4357/abb476
                ce176a90-03d4-4b2f-b342-614d5b04a7c0
                © 2020

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