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Neutrino emission from the direction of the blazar TXS 0506+056 prior to the IceCube-170922A alert
Journal article   Open access   Peer reviewed

Neutrino emission from the direction of the blazar TXS 0506+056 prior to the IceCube-170922A alert

Maryon Ahrens, Christian Bohm, Jonathan P. Dumm, Chad Finley, Samuel Flis, Klas Hultqvist, Erin O'Sullivan, Christian Walck and IceCube Collaboration
Science (American Association for the Advancement of Science), v 361(6398), pp 147-151
2018
PMID: 30002248
url
http://arxiv.org/abs/1807.08794View

Abstract

Fysik Naturvetenskap ESI Highly Cited Paper (Incites) Natural Sciences Physical Sciences
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 3.5 sigma 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.

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Domestic collaboration
International collaboration
Web of Science research areas
Astronomy & Astrophysics
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