The optical detection unit for Baikal-GVD neutrino telescope

A.D. Avrorin,A.V. Avrorin,V. Aynutdinov,R. Bannash,I. A. Belolaptikov,D. Yu. Bogorodsky,V. Brudanin,Nikolay M. Budnev,I. Danilchenko,G. V. Domogatsky,A. A. Doroshenko,A. Dyachok,Zh.-A. Dzhilkibaev,S. V. Fialkovsky,A. Gafarov,O. N. Gaponenko,K. Golubkov,T. Gress,Z. Honz,Konstantin Kebkal,O.G. Kebkal,K. Konischev,E. Konstantinov,A.V. Korobchenko,A. P. Koshechkin,F.K. Koshel,A.V. Kozhin,V. F. Kulepov,D. A. Kuleshov,V.I. Ljashuk,M. B. Milenin,R. R. Mirgazov,E.R. Osipova,A. I. Panfilov,L. Pankov,A. A. Perevalov,E. Pliskovsky,M. I. Rozanov,V. Yu. Rubtzov,E.V. Rjabov,B.A. Shaybonov,A. Sheifler,A.V. Skurihin,A.A. Smagina,O. V. Suvorova,V. Tabolenko,B. Tarashansky,S. A. Yakovlev,A. Zagorodnikov,V. Zhukov,V. L. Zurbanov

The optical detection unit for Baikal-GVD neutrino telescope

2016

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.

Keywords:

Calibration
Neutrino
Telescope
Astrophysics
Physics
neutrino telescope

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