Speaker
Bair Shaybonov
(JINR)
Description
The first stage of the Baikal-GVD neutrino telescope will be composed of more than two thousand light sensors, Optical Modules (OMs), installed deep underwater in Lake Baikal. We describe developed calibration methods which use OM LEDs, the calibration laser source, atmospheric muons etc. and discuss the performance of these methods.
Registration number following "ICRC2015-I/" | 893 |
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Collaboration | -- not specified -- |
Primary author
Bair Shaybonov
(JINR)