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

MPS-Authors

IceCube collaboration, 
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Fermi-LAT collaboration, 
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

MAGIC collaboration, 
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

AGILE, 
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

ASAS-SN, 
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

HAWC, 
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

S,  H. E. S.
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

INTEGRAL, 
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Kanata, 
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Kiso, 
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Kapteyn, 
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

telescope,  Liverpool
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Subaru, 
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

Swift/NuSTAR, 
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

VERITAS, 
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

VLA/17B-403, 
Max Planck Institute for Physics, Max Planck Society and Cooperation Partners;

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Citation

IceCube collaboration, Fermi-LAT collaboration, MAGIC collaboration, AGILE, ASAS-SN, HAWC, et al. (2018). Multi-messenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A. Science Magazine, (361), 1378. Retrieved from https://publications.mppmu.mpg.de/?action=search&mpi=MPP-2018-385.


Cite as: https://hdl.handle.net/21.11116/0000-0003-F897-B
Abstract
Individual astrophysical sources previously detected in 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 approximately 290 TeV. Its arrival direction was consistent with the location of a known gamma-ray blazar TXS 0506+056, observed to be in a flaring state. An extensive multi-wavelength campaign followed, ranging from radio frequencies to gamma-rays. These observations characterize the variability and energetics of the blazar and include the first detection of TXS 0506+056 in very-high-energy gamma-rays. This observation of a neutrino in spatial coincidence with a gamma-ray emitting blazar during an active phase suggests that blazars may be a source of high-energy neutrinos.