PoS - Proceedings of Science
Volume 301 - 35th International Cosmic Ray Conference (ICRC2017) - Session Neutrino. NU-instrumentation
Status of the Baikal-GVD experiment - 2017
V. Aynutdinov,* A.D. Avrorin, A.V. Avrovin, R. Bannash, I. Belolaptikov, V. Brudanin, N.M. Budnev, I. Danilchenko, G. Domogatsky, A. Doroshenko, R. Dvornicky, A.N. Dyachok, Z. Dzhilkibaev, L. Fajt, S. Fialkovsky, A. Gafarov, K. Golubkov, T. Gress, Z. Hons, K. Kebkal, O. Kebkal, M.M. Kolbin, K. Konischev, A.V. Korobchenko, A. Koshechkin, F. Koshel, V. Kozhin, V. Kulepov, D. Kuleshov, M. Milenin, R. Mirgazov, E. Osipova, A. Panfilov, L. Pankov, D. Petukhov, E.N. Pliskovsky, M. Rozanov, E.V. Rjabov, G. Safronov, B. Shaybonov, M. Shelepov, F. Simkovic, A.V. Skurihin, I. Stekl, O. Suvorova, V.A. Tabolenko, B. Tarashansky, S. Yakovlev, A. Zagorodnikov, V. Zurbanov
*corresponding author
Full text: pdf
Pre-published on: August 16, 2017
Published on: August 03, 2018
Abstract
Baikal-GVD is a kilometer scale neutrino telescope under construction in Lake Baikal, which will be formed by multimegaton subarrays – clusters of strings. First demonstration cluster “Dubna” has been deployed in 2015 and comprises 192 optical modules (OMs). In 2016 cluster “Dubna” was upgraded to baseline configuration which comprises 288 OMs arranged at eight strings. The second full scale GVD-cluster was deployed and put in operation in 2017 in Lake Baikal. We review a present activity towards the GVD implementation and discuss some selected results obtained with array “Dubna”.
DOI: https://doi.org/10.22323/1.301.1034
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