Abstract
The Baikal collaboration is building the next generation Gigaton-scale deep underwater neutrino telescope in Lake Baikal. Its goal is to discover and observe high-energy (E > 100 GeV) neutrino sources in the Universe. Since April 2018 the telescope is operating in a configuration of three subarrays of optical modules (OMs) with 864 OMs on 24 vertical strings in total. We present the status of the experiment and first results obtained from data taken 2015 - 2017.
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