Search for neutrino bursts from core collapse supernovae at the Baksan Underground Scintillation Telescope
R.V. Novoseltseva, M.M. Boliev, I.M. Dzaparova, M.M. Kochkarov, S.P., Mikheyev, Yu.F. Novoseltsev, V.B. Petkov, P.S. Striganov, G.V. Volchenko,, V.I. Volchenko, A.F. Yanin

TL;DR
This paper reports on a 24.7-year experiment using the Baksan Underground Scintillation Telescope to detect neutrino bursts from supernovae, setting an upper limit on supernova collapse frequency in our galaxy.
Contribution
It provides long-term observational data and constraints on supernova neutrino burst frequency in our galaxy.
Findings
No neutrino burst detections over 24.7 years
Upper bound of 0.093 supernovae per year in our galaxy
Extended observational period improves constraints on supernova rates
Abstract
Current status and results of the experiment on recording neutrino bursts are presented. The observation time (since 1980) is 24.7 years. The upper bound of collapse frequency in our Galaxy is 0.093 (90% CL).
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astrophysics and Cosmic Phenomena · Neutrino Physics Research
