/ Instrumentation


The optical detection unit for Baikal-GVD neutrino telescope


Avrorin, A.D. (Moscow, INR) ; Avrorin, A.V. (Moscow, INR) ; Aynutdinov, V.M. (Moscow, INR) ; Bannash, R. (BESSY, Berlin) ; Belolaptikov, I.A. (Dubna, JINR) ; Bogorodsky, D.Yu. (Irkutsk State U.) ; Brudanin, V.B. (Dubna, JINR) ; Budnev, N.M. (Irkutsk State U.) ; Danilchenko, I.A. (Moscow, INR) ; Domogatsky, G.V. (Moscow, INR) ; Doroshenko, A.A. (Moscow, INR) ; Dyachok, A.N. (Irkutsk State U.) ; Dzhilkibaev, Zh.A.M. (Moscow, INR) ; Fialkovsky, S.V. (Nizhnii Novgorod State Tech. U.) ; Gafarov, A.R. (Irkutsk State U.) ; Gaponenko, O.N. (Moscow, INR) ; Golubkov, K.V. (Moscow, INR) ; Gress, T.I. (Irkutsk State U.) ; Honz, Z. (Dubna, JINR) ; Kebkal, K.G. (BESSY, Berlin) ; Kebkal, O.G. (BESSY, Berlin) ; Konischev, K.V. (Dubna, JINR) ; Konstantinov, E.N. (Irkutsk State U.) ; Korobchenko, A.V. (Irkutsk State U.) ; Koshechkin, A.P. (Moscow, INR) ; Koshel, F.K. (Moscow, INR) ; Kozhin, A.V. (SINP, Moscow) ; Kulepov, V.F. (Nizhnii Novgorod State Tech. U.) ; Kuleshov, D.A. (Moscow, INR) ; Ljashuk, V.I. (Moscow, INR) ; Milenin, M.B. (Nizhnii Novgorod State Tech. U.) ; Mirgazov, R.A. (Irkutsk State U.) ; Osipova, E.R. (SINP, Moscow) ; Panfilov, A.I. (Moscow, INR) ; Pan'kov, L.V. (Irkutsk State U.) ; Perevalov, A.A. (Irkutsk State U.) ; Pliskovsky, E.N. (Dubna, JINR) ; Rozanov, M.I. (St. Petersburg, Marine Tech U.) ; Rubtzov, V.Yu. (Irkutsk State U.) ; Rjabov, E.V. (Irkutsk State U.) ; Shaybonov, B.A. (Dubna, JINR) ; Sheifler, A.A. (Moscow, INR) ; Skurihin, A.V. (SINP, Moscow) ; Smagina, A.A. (Dubna, JINR) ; Suvorova, O.V. (Moscow, INR) ; Tabolenko, V.A. (Irkutsk State U.) ; Tarashansky, B.A. (Irkutsk State U.) ; Yakovlev, S.A. (BESSY, Berlin) ; Zagorodnikov, A.V. (Irkutsk State U.) ; Zhukov, V.A. (Moscow, INR) ; Zurbanov, V.L. (Irkutsk State U.)

Published in: EPJ Web Conf.
Year: 2016
Vol.: 121
Page No: 05008
Pages: 6
Year: 2016-07-06 published

Abstract: The first stage of the GVD-cluster composed of five strings was deployed in April 2014. Each string consists of two sections with 12 optical modules per section. A section is the basic detection unit of the Baikal neutrino telescope. We will describe the section design, review its basic elements - optical modules, FADC readout units, slow control and calibration systems, and present selected results for section in-situ tests in Lake Baikal.

Web-Page: http://inspirehep.net/record/1475963/files/epjconf-RICAP-14_05008.pdf

Total numbers of views: 184
Numbers of unique views: 80
DOI: 10.1051/epjconf/201612105008
 Record created 2016-08-04, last modified 2016-08-04


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