PoS - Proceedings of Science
Volume 301 - 35th International Cosmic Ray Conference (ICRC2017) - Session Neutrino. NU-astrophysical neutrinos
Search for astrophysical sources of muon neutrinos with 38 years of data from the BUST detector
M. Kochkarov*, M.M. Boliev, I.M. Dzaparova, R.V. Novoseltseva, V.B. Petkova, P.S. Striganov, V. Volchenko, A.F. Yanin and A.V. Butkevich
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Pre-published on: August 16, 2017
Published on: August 03, 2018
Baksan Underground Scintillation Telescope is an underground detector located at the Northern Caucasus (Russia). The BUST can detect an astrophysical flux of neutrinos from Galactic sources as an excess of cosmic ray muon neutrinos arriving from the source direction. The search performed using 38 years (live time = 30.9) of the BUST dataset to look for a statistically significant excess of events arriving within a solid angle. No significant excess of events produced by astrophysical sources is found. Since the number of detected events is compatible with the number of expected background events upper limit on the muon neutrino flux is determined.
DOI: https://doi.org/10.22323/1.301.0943
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