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  • Baikal-GVD: status and pros...
    Avrorin, A.D.; Avrorin, A.V.; Aynutdinov, V.M.; Bannash, R.; Belolaptikov, I.A.; Brudanin, V.B.; Budnev, N.M.; Doroshenko, A.A.; Domogatsky, G.V.; Dvornický, R.; Dyachok, A.N.; Dzhilkibaev, Zh.-A.M.; Fajt, L.; Fialkovsky, S.V.; Gafarov, A.R.; Golubkov, K.V.; Gres, T.I.; Honz, Z.; Kebkal, K.G.; Kebkal, O.G.; Khramov, E.V.; Kolbin, M.M.; Konischev, K.V.; Korobchenko, A.P.; Koshechkin, A.P.; Kozhin, V.A.; Kulepov, V.F.; Kuleshov, D.A.; Milenin, M.B.; Mirgazov, R.A.; Osipova, E.R.; Panfilov, A.I.; Pan’kov, L.V.; Petukhov, D.P.; Pliskovsky, E.N.; Rozanov, M.I.; Rjabov, E.V.; Rushay, V.D.; Safronov, G.B.; Simkovic, F.; Shoibonov, B.A.; Solovjev, A.G.; Sorokovikov, M.N.; Shelepov, M.D.; Suvorova, O.V.; Shtekl, I.; Tabolenko, V.A.; Tarashansky, B.A.; Yakovlev, S.A.; Zagorodnikov, A.V.; Zurbanov, V.L.

    EPJ Web of Conferences, 01/2018, Letnik: 191
    Journal Article, Conference Proceeding

    Baikal-GVD is a next generation, kilometer-scale neutrino telescope under construction in Lake Baikal. It is designed to detect astrophysical neutrino fluxes at energies from a few TeV up to 100 PeV. GVD is formed by multi-megaton subarrays (clusters). The array construction started in 2015 by deployment of a reduced-size demonstration cluster named "Dubna" . The first cluster in it’s baseline configuration was deployed in 2016, the second in 2017 and the third in 2018. The full-scale GVD will be an array of ~10.000 light sensors with an instrumented volume about of 2 cubic km. The first phase (GVD-1) is planned to be completed by 2020-2021. It will comprise 8 clusters with 2304 light sensors in total. We describe the design of Baikal-GVD and present selected results obtained in 2015 - 2017.