Follow up of the IceCube alerts with the Baikal-GVD telescope

The high-energy muon neutrino events of the IceCube telescope, that are triggered as neutrino alerts in one of two probability ranks of astrophysical origin, "gold" and "bronze", have been followed up by the Baikal-GVD in a fast quasi-online mode since September 2020. Search for...

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Published inarXiv.org
Main Authors Allakhverdyan, V A, Avrorin, A D, Avrorin, A V, Aynutdinov, V M, Bannasch, R, Bardačová, Z, Belolaptikov, I A, Borina, I V, Brudanin, V B, Budnev, N M, Dik, V Y, Domogatsky, G V, Doroshenko, A A, Dvornický, R, Dyachok, A N, Zh -A M Dzhilkibaev, Eckerová, E, Elzhov, T V, Fajt, L, Fialkovski, S V, Gafarov, A R, Golubkov, K V, Gorshkov, N S, Gress, T I, Katulin, M S, Kebkal, K G, Kebkal, O G, Khramov, E V, Kolbin, M M, Konischev, K V, Kopański, K A, Korobchenko, A V, Koshechkin, A P, Kozhin, V A, Kruglov, M V, Kryukov, M K, Kulepov, V F, Malecki, Pa, Malyshkin, Y M, Milenin, M B, Mirgazov, R R, Naumov, D V, Nazari, V, Noga, W, Petukhov, D P, Pliskovsky, E N, Rozanov, M I, Rushay, V D, Ryabov, E V, Safronov, G B, Shaybonov, B A, Shelepov, M D, Šimkovic, F, Sirenko, A E, Skurikhin, A V, Solovjev, A G, Sorokovikov, M N, Štekl, I, Stromakov, A P, Sushenok, E O, Suvorova, O V, Tabolenko, V A, Tarashansky, B A, Yablokova, Y V, Yakovlev, S A, Zaborov, D N, the Baikal-GVD Collaboration
Format Paper Journal Article
LanguageEnglish
Published Ithaca Cornell University Library, arXiv.org 18.09.2021
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Summary:The high-energy muon neutrino events of the IceCube telescope, that are triggered as neutrino alerts in one of two probability ranks of astrophysical origin, "gold" and "bronze", have been followed up by the Baikal-GVD in a fast quasi-online mode since September 2020. Search for correlations between alerts and GVD events reconstructed in two modes, muon-track and cascades (electromagnetic or hadronic showers), for the time windows \( \pm \) 1 h and \( \pm \) 12 h does not indicate statistically significant excess of the measured events over the expected number of background events. Upper limits on the neutrino fluence will be presented for each alert.
ISSN:2331-8422
DOI:10.48550/arxiv.2107.14303