Calibration and monitoring units of the Baikal-GVD neutrino telescope

Avrorin, А.D.; Avrorin, A.V.; Aynutdinov, V. M.; Баннаш, Р.; Белолаптиков, И. А.; Brudanin, V.; Буднев, Н. М.; Danilchenko, I. A.; Domogatsky, G. V.; Dvornický, R.; Dyachok, A. N.; Dzhilkibaev, Zhan; Fajt, L.; Fialkovsky, S.V.; Гафаров, А. Р.; Golubkov, K.V.; Дорошенко, А. А.; Гресс, Т.; Honz, Z.; Кебкал, К.Г.; Kebkal, O.G.; Kolbin, M.M.; Konischev, K. V.; Коробченко, А. В.; Кошечкин, А. П.; Koshel, F.K.; Kozhin, A.V.; Kulepov, V.F.; Kuleshov, D.A.; Milenin, M. V.; Mirgazov, R.; Osipova, E.R.; Панфилов, А. И.; Pankov, L.; Петухов, Д. П.; Pliskovsky, E. N.; Rozanov, M.I.; Rjabov, E.V.; Safronov, G.; Shaybonov, B. A.; Shelepov, M.D.; Šimkovic, F.; Skurihin, Aleksandr Vasilevich; Štekl, I.; Суворова, О. В.; Таболенко, В. А.; Tarashansky, B.; Yakovlev, S. A.; Загородников, А.; Зурбанов, В. Л.

doi:10.22323/1.301.1032

Cited by 2 publications

(1 citation statement)

References 7 publications

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“…The online monitoring system of the telescope is designed for the continuos registration of the measurement conditions for each OM. For more details see [6]. Here, we put emphasis on the photo-multiplier noise rate only, which is the subject of our interest.…”

Section: Noise Monitoring Systemmentioning

confidence: 99%

The optical noise monitoring systems of the Lake Baikal environment for the Baikal-GVD telescope

Dvornický¹,

Avrorin²,

Avrorin³

et al. 2019

Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)

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We present data on the luminescence of the Baikal water medium collected with the Baikal-GVD neutrino telescope. This three-dimensional array of light sensors allows the observation of time and spatial variations of the ambient light field. We report on observation of an increase of luminescence activity in 2016 and 2018. On the contrary, we observed practically constant optical noise in 2017. An agreement has been found between two independent optical noise data sets. These are data collected with online monitoring system and the trigger system of the cluster.

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Section: Noise Monitoring Systemmentioning

confidence: 99%

The optical noise monitoring systems of the Lake Baikal environment for the Baikal-GVD telescope

Dvornický¹,

Avrorin²,

Avrorin³

et al. 2019

Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)

Self Cite

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High-Energy Neutrino Astronomy—Baikal-GVD Neutrino Telescope in Lake Baikal

et al. 2021

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High-energy neutrino astronomy is a fascinating new field of research, rapidly developing over recent years. It opens a new observation window on the most violent processes in the universe, fitting very well to the concept of multi-messenger astronomy. This may be exemplified by the recent discovery of the high-energy neutrino emissions from the γ-ray loud blazar TXS 0506+056. Constraining astrophysical neutrino fluxes can also help to understand the long-standing mystery of the origin of the ultra-high energy cosmic rays. Astronomical studies of high-energy neutrinos are carried out by large-scale next-generation neutrino telescopes located in different regions of the world, forming a global network of complementary detectors. The Baikal-GVD, being currently the largest neutrino telescope in the Northern Hemisphere and still growing up, is an important constituent of this network. This paper briefly reviews working principles, analysis methods, and some selected results of the Baikal-GVD neutrino telescope.

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Calibration and monitoring units of the Baikal-GVD neutrino telescope

Cited by 2 publications

References 7 publications

The optical noise monitoring systems of the Lake Baikal environment for the Baikal-GVD telescope

The optical noise monitoring systems of the Lake Baikal environment for the Baikal-GVD telescope

High-Energy Neutrino Astronomy—Baikal-GVD Neutrino Telescope in Lake Baikal

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