EPJ Web of Conferences
Volume 116, 2016Very Large Volume Neutrino Telescope (VLVnT-2015)
|Number of page(s)||5|
|Section||Photon Detection Technique|
|Published online||11 April 2016|
The optical module of Baikal-GVD
1 Institute for Nuclear Research, 60th October Anniversary pr. 7A, Moscow 117312, Russia
2 Joint Institute for Nuclear Research, Dubna 141980, Russia
3 Irkutsk State University, Irkutsk 664003, Russia
4 Skobeltsyn Institute of Nuclear Physics MSU, Moscow 119991, Russia
5 Nizhni Novgorod State Technical University, Nizhni Novgorod 603950, Russia
6 St. Petersburg State Marine University, St. Petersburg 190008, Russia
7 EvoLogics GmbH, Berlin, Germany
Published online: 11 April 2016
The Baikal-GVD neutrino telescope in Lake Baikal is intended for studying astrophysical neutrino fluxes by recording the Cherenkov radiation of the secondary muons and showers generated in neutrino interactions. The first stage of Baikal-GVD will be equipped with about 2300 optical modules. We describe the design of the optical module, the front-end electronics and the laboratory characterization and calibration before deployment.
© Owned by the authors, published by EDP Sciences, 2016
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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