EPJ Web of Conferences
Volume 121, 2016Roma International Conference on Astroparticle Physics 2014 (RICAP-14)
|Number of page(s)||6|
|Section||High Energy Neutrinos|
|Published online||06 July 2016|
The optical detection unit for Baikal-GVD neutrino telescope
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
a Corresponding author: email@example.com
Published online: 6 July 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.
© The Authors, published by EDP Sciences
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.