The results of three different searches for neutrino candidates, associated with the IceCube-170922A event or from the direction of TXS 0506+056, by the ANTARES neutrino telescope, are presented. The first search refers to the online follow-up of the IceCube alert; the second is based on the standard time-integrated method employed by the Collaboration to search for point-like neutrino sources; the third uses information from the IceCube time-dependent analysis that reported bursting activity centered on 2014 December 13, as input for an ANTARES time-dependent analysis. The online follow-up and the time-dependent analysis yield no events related to the source. The timeintegrated study performed over a period from 2007 to 2017 fits 1.03 signal events, which corresponds to a p-value of 3.4% (not considering trial factors). Only for two other astrophysical objects in our candidate list has a smaller p-value been found. When considering that 107 sources have been investigated, the post-trial p-value for TXS 0506+056 corresponds to 87%.

Albert, A., André, M., Anghinolfi, M., Anton, G., Ardid, M., Aubert, J., et al. (2018). The Search for Neutrinos from TXS 0506+056 with the ANTARES Telescope. THE ASTROPHYSICAL JOURNAL LETTERS, 863(2), 1-6 [10.3847/2041-8213/aad8c0].

The Search for Neutrinos from TXS 0506+056 with the ANTARES Telescope

Chiarusi, T.;Donà, R.;Fusco, L.;Illuminati, G.;Margiotta, A.;Spurio, M.;Versari, F.;
2018

Abstract

The results of three different searches for neutrino candidates, associated with the IceCube-170922A event or from the direction of TXS 0506+056, by the ANTARES neutrino telescope, are presented. The first search refers to the online follow-up of the IceCube alert; the second is based on the standard time-integrated method employed by the Collaboration to search for point-like neutrino sources; the third uses information from the IceCube time-dependent analysis that reported bursting activity centered on 2014 December 13, as input for an ANTARES time-dependent analysis. The online follow-up and the time-dependent analysis yield no events related to the source. The timeintegrated study performed over a period from 2007 to 2017 fits 1.03 signal events, which corresponds to a p-value of 3.4% (not considering trial factors). Only for two other astrophysical objects in our candidate list has a smaller p-value been found. When considering that 107 sources have been investigated, the post-trial p-value for TXS 0506+056 corresponds to 87%.
2018
Albert, A., André, M., Anghinolfi, M., Anton, G., Ardid, M., Aubert, J., et al. (2018). The Search for Neutrinos from TXS 0506+056 with the ANTARES Telescope. THE ASTROPHYSICAL JOURNAL LETTERS, 863(2), 1-6 [10.3847/2041-8213/aad8c0].
Albert, A.; André, M.; Anghinolfi, M.; Anton, G.; Ardid, M.; Aubert, J.-J.; Aublin, J.; Avgitas, T.; Baret, B.; Barrios-Martí, J.; Basa, S.; Belhorma,...espandi
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/641364
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