Neutrino astronomy at Lake Baikal
Dmitry Zaborov (for the Baikal-GVD Collaboration)

TL;DR
This paper reviews recent advancements in high-energy neutrino astronomy, focusing on the Baikal-GVD telescope's current status and its recent observations of atmospheric and astrophysical neutrinos, highlighting progress in the field.
Contribution
It provides an update on the Baikal-GVD neutrino telescope's development and recent findings, contributing new observational data from Lake Baikal.
Findings
Detection of atmospheric neutrinos
Observation of astrophysical neutrinos
Progress in neutrino telescope technology
Abstract
High energy neutrino astronomy has seen significant progress in the past few years. This includes the detection of neutrino flux from the Galactic plane, as well as strong evidence for neutrino emission from the active galaxy NGC 1068, both reported by IceCube. New results start coming from the two km-scale neutrino telescopes under construction in the Northern hemisphere: KM3NeT in the Mediterranean Sea and Baikal-GVD in Lake Baikal. After briefly reviewing the status of the field, we present the current status of the Baikal-GVD neutrino telescope and its recent results, including observations of atmospheric and astrophysical neutrinos.
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