Optical Observations Reveal Strong Evidence for High-energy Neutrino Progenitor

Lipunov, V. M.; Kornilov, V. G.; Zhirkov, K.; Gorbovskoy, E.; Budnev, N. M.; Buckley, D. A. H.; Rebolo, R.; Serra-Ricart, M.; Podesta, R.; Tyurina, N.; Gress, O.; Sergienko, Y.; 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.; Van Soelen, B.; Razzaque, S.; Böttcher, M.
Referencia bibliográfica

The Astrophysical Journal

Fecha de publicación:
6
2020
Número de autores
35
Número de autores del IAC
2
Número de citas
19
Número de citas referidas
11
Descripción
We present the earliest astronomical observation of a high-energy neutrino error box of which the variability was discovered after high-energy-neutrino detection. The one robotic telescope of the MASTER global international networks automatically imaged the error box of the very high-energy-neutrino event IceCube-170922A. Observations were carried out in minutes 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 50σ significance level. We also present own a unique 16 yr light curve of blazar TXS 0506+056 (518 data set).