2016
DOI: 10.1051/epjconf/201611611005
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Baikal-GVD: Results, status and plans

Abstract: Abstract. The future next-generation neutrino telescope Baikal-GVD will be a km3-scale array aimed at the detection of astrophysical neutrino fluxes. It will have modular structure and consist of functionally independent sub-arrays -clusters of strings of optical modules. The prototyping phase of the project has been concluded in 2015 with the deployment of the first cluster of Baikal-GVD in Lake Baikal. We discuss the current status and perspectives of the Baikal-GVD project.

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Cited by 5 publications
(3 citation statements)
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“…The configuration of the ICS (see Fig. 3) is basically identical to the conventional Baikal-GVD strings configuration [4]. The ICS consists of three sections of OMs.…”
Section: Technical Implementation Of the Intercluster Stringmentioning
confidence: 95%
“…The configuration of the ICS (see Fig. 3) is basically identical to the conventional Baikal-GVD strings configuration [4]. The ICS consists of three sections of OMs.…”
Section: Technical Implementation Of the Intercluster Stringmentioning
confidence: 95%
“…It was followed by the BAIKAL detector in the water of Lake Baikal [11], the AMANDA detector deployed in the glacial ice at the South Pole [12] and the ANTARES detector in the Mediterranean Sea [13]. Based on the success of these projects the larger IceCube detector was built at the South Pole [14], KM3NeT is being built in the Mediterranean Sea [15] and Baikal GVD is under construction in Lake Baikal [16].…”
Section: Existing Neutrino Telescopesmentioning
confidence: 99%
“…In lake Baikal the new detector Baikal GVD (Gigaton Volume Detector) [16] aiming at the 1 TeV to 10 6 TeV neutrino energy regime, is in the first phase of construction with two out of the planned 8 clusters of strings being deployed. The first phase will cover a volume of 0.4 km 3 , the final size with 27 clusters should reach a volume of 1.5 km 3 .…”
Section: Future Neutrino Telescopesmentioning
confidence: 99%