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SUMMARY:Preliminary estimation of the Baikal-GVD detector sensitivity to d
 iffuse astrophysical neutrino flux in track-like event analysis
DTSTART;VALUE=DATE-TIME:20261027T162500Z
DTEND;VALUE=DATE-TIME:20261027T163000Z
DTSTAMP;VALUE=DATE-TIME:20261019T232922Z
UID:indico-contribution-6427@cern.ch
DESCRIPTION:Speakers: Daria Busel (NRNU MEPhI)\nThe Baikal-GVD neutrino te
 lescope is situated in Lake Baikal at depths of $750$ – $1275$  m. Its c
 urrent instrumented volume is $0.8$ km$^{3}$\, and it is being expanded to
 ward $1$ km$^{3}$. Baikal-GVD is capable of detecting neutrinos in TeV-PeV
  energy range\, including those of astrophysical origin. Previously Baikal
 -GVD has demonstrated an observation of astrophysical neutrino flux in the
  cascade detection channel. Present work focuses on development of likelih
 ood-based analysis technique aimed at the diffuse astrophysical neutrino f
 lux search using muon track detection channel. Preliminary results on its 
 sensitivity analysis are presented.\n\nhttps://indico.particle.mephi.ru/ev
 ent/626/contributions/6427/
LOCATION:Sevastopol hotel Conference Hall 1
URL:https://indico.particle.mephi.ru/event/626/contributions/6427/
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