Muon Track Reconstruction Procedures at the Baikal-GVD Neutrino Telescope
Grigory Safronov

TL;DR
The paper details the Baikal-GVD neutrino telescope's muon track reconstruction methods, achieving high directional accuracy and presenting preliminary results from 2019-2021 data analysis.
Contribution
It introduces new track reconstruction procedures and analysis pipelines for neutrino detection at the Baikal-GVD telescope.
Findings
Muon track reconstruction achieves up to 0.2 degree directional precision.
Analysis pipeline applied to 2019-2021 data yields preliminary neutrino event results.
Methods improve neutrino candidate selection and energy estimation.
Abstract
The Baikal-GVD neutrino telescope is the largest neutrino detector of its kind in the Northern Hemisphere. Muons produced in neutrino interaction in the vicinity of the detector leave track-like response in the detector allowing to reconstruct the neutrino arrival direction with the precision up to 0.2 degree. The Baikal-GVD collaboration has developed a variety of methods for the track-like event analysis. Methods for track-like event direction and energy reconstruction and neutrino cadidate event selection are discussed in this report. Preliminary results of application of analysis pipeline to the data-taking seasons from 2019 to 2021 are shown.
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