Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/117727
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Type: Journal article
Title: Neutrino emission from the direction of the blazar TXS 0506+056 prior to the IceCube-170922A alert
Author: Aartsen, M.G.
Ackermann, M.
Adams, J.
Aguilar, J.A.
Ahlers, M.
Ahrens, M.
Al Samarai, I.
Altmann, D.
Andeen, K.
Anderson, T.
Ansseau, I.
Anton, G.
Arguelles, C.
Arsioli, B.
Auffenberg, J.
Axani, S.
Bagherpour, H.
Bai, X.
Barron, J.P.
Barwick, S.W.
et al.
Citation: Science, 2018; 361(6398):147-151
Publisher: American Association for the Advancement of Science
Issue Date: 2018
ISSN: 0036-8075
1095-9203
Statement of
Responsibility: 
M.G. Aartsen … G.C. Hill .. A. Kyriacou … S. Robertson … A. Wallace … B.J. Whelan … [et al.] (The IceCube Collaboration)
Abstract: A high-energy neutrino event detected by IceCube on 22 September 2017 was coincident in direction and time with a gamma-ray flare from the blazar TXS 0506+056. Prompted by this association, we investigated 9.5 years of IceCube neutrino observations to search for excess emission at the position of the blazar. We found an excess of high-energy neutrino events, with respect to atmospheric backgrounds, at that position between September 2014 and March 2015. Allowing for time-variable flux, this constitutes 3.5σ evidence for neutrino emission from the direction of TXS 0506+056, independent of and prior to the 2017 flaring episode. This suggests that blazars are identifiable sources of the high-energy astrophysical neutrino flux.
Keywords: IceCube Collaboration
Rights: © 2018 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works. http://www.sciencemag.org/about/science-licenses-journal-article-reuseThis is an article distributed under the terms of the Science Journals Default License.
DOI: 10.1126/science.aat2890
Grant ID: ARC
Published version: http://dx.doi.org/10.1126/science.aat2890
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