Baikal-GVD Document 27-v1

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High-energy neutrino-induced cascade from the direction of the flaring radio blazar TXS 0506+056 observed by the Baikal Gigaton Volume Detector in 2021

Document #:
Baikal-GVD-doc-27-v1
Document type:
Paper
Submitted by:
Yury Malyshkin
Updated by:
Yury Malyshkin
Document Created:
11 Oct 2022, 18:45
Contents Revised:
11 Oct 2022, 18:45
Metadata Revised:
11 Oct 2022, 18:45
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Abstract:
The existence of high-energy astrophysical neutrinos has been unambiguously demonstrated, but their sources remain elusive. IceCube reported an association of a 290-TeV neutrino with a gamma-ray flare of TXS 0506+056, an active galactic nucleus with a compact radio jet pointing to us. Later, radio blazars were shown to be associated with IceCube neutrino events with high statistical significance. These associations remained unconfirmed with the data of independent experiments. Here we report on the detection of a rare neutrino with the estimated energy of 224 TeV from the direction of TXS 0506+056 by the new Baikal-GVD neutrino telescope in April 2021 followed by a radio flare observed by RATAN-600. This event is the highest-energy cascade detected so far by Baikal-GVD from a direction below horizon. The result supports previous observations that radio blazars in general, and TXS 0506+056 in particular, are sources of high-energy neutrinos, and opens up the cascade channel for the neutrino astronomy.
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