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Optical Observations Reveal Strong Evidence for High Energy Neutrino Progenitor

We present the earliest astronomical observation of a high energy neutrino error box in which its variability was discovered after high-energy neutrinos detection. The one robotic telescope of the MASTER global international network (Lipunov et al. 2010) automatically imaged the error box of the ver...

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Published in:arXiv.org 2020-06
Main Authors: Lipunov, V M, Kornilov, V G, Zhirkov, K K, Gorbovskoy, E S, Budnev, N M, Buckley, D A H, Rebolo, R, Serra-Ricart, M, Podesta, R, Tyurina, N, Gress, O, Sergienko, Yu, Yurkov, V, Gabovich, A, Balanutsa, P, Gorbunov, I, Vlasenko, D, Balakin, F, Topolev, V, Pozdnyakov, A, Kuznetsov, A, Vladimirov, V, Chasovnikov, A, Kuvshinov, D, Grinshpun, V, Minkina, E, Petkov, V B, Svertilov, S I, Lopez, C, Podesta, F, Levato, H, Tlatov, A, B van Soelen, Razzaque, S, Böttcher, M
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Language:English
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Summary:We present the earliest astronomical observation of a high energy neutrino error box in which its variability was discovered after high-energy neutrinos detection. The one robotic telescope of the MASTER global international network (Lipunov et al. 2010) automatically imaged the error box of the very high-energy neutrino event IceCube-170922A. Observations were carried out in minute after the IceCube-170922A neutrino event was detected by the IceCube observatory at the South Pole. MASTER found the blazar TXS 0506+056 to be in the off-state after one minute and then switched to the on-state no later than two hours after the event. The effect is observed at a 50-sigma significance level. Also we present own unique 16-years light curve of blazar TXS 0506+056 (518 data set).
ISSN:2331-8422
DOI:10.48550/arxiv.2006.04918