2022
DOI: 10.1016/j.nima.2022.167047
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TAIGA—A hybrid array for high energy gamma-ray astronomy and cosmic-ray physics

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Cited by 5 publications
(4 citation statements)
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“…Then in 2012 we finished deployment of the Tunka-133 array consisting of 175 Cherenkov detectors [7,8] arranged over an area of 3 km 2 . In 2022, we completed the deployment and commissioning of the TAIGA-1 hybrid complex [9,10]. It consists of 120 TAIGA-HiSCORE wide-angle Cherenkov stations, three 4-m class Imaging Atmospheric Cherenkov Telescopes (IACT) and 250 m 2 of scintillation particle detectors of Tunka-Grande [11] and TAIGA-MUON [12] arrays.…”
Section: The Tunka Valley Experimental Facilitymentioning
confidence: 99%
“…Then in 2012 we finished deployment of the Tunka-133 array consisting of 175 Cherenkov detectors [7,8] arranged over an area of 3 km 2 . In 2022, we completed the deployment and commissioning of the TAIGA-1 hybrid complex [9,10]. It consists of 120 TAIGA-HiSCORE wide-angle Cherenkov stations, three 4-m class Imaging Atmospheric Cherenkov Telescopes (IACT) and 250 m 2 of scintillation particle detectors of Tunka-Grande [11] and TAIGA-MUON [12] arrays.…”
Section: The Tunka Valley Experimental Facilitymentioning
confidence: 99%
“…Then in 2012 we finished deployment of the Tunka-133 array consisting of 175 Cherenkov detectors [7,8] arranged over an area of 3 km 2 . In 2022, we completed the deployment and commission of the TAIGA-1 hybrid complex [9,10]. It consists of 120 TAIGA-HiSCORE wide-angle Cherenkov stations, three 4-m class Imaging Atmospheric Cherenkov Telescopes (IACT) and 250 m 2 of scintillation particle detectors of Tunka-Grande [11] and TAIGA-MUON [12] arrays.…”
Section: The Tunka Valley Experimental Facilitymentioning
confidence: 99%
“…The TAIGA Astrophysical complex (Tunka Advanced Instrument for cosmic ray and Gamma Astronomy) [4] is designed to study gamma radiation and charged cosmic rays in the energy range of 10 13 − 10 18 eV. The complex includes installations aimed both at studying charged cosmic rays: Tunka-133 [5], Tunka-Grande [6], and for gamma-ray astronomy in the TeV-PeV energy range: TAIGA-Muon [6], TAIGA-HiSCORE [7] and TAIGA-IACT [8]. The TAIGA-IACT installation consists of three atmospheric Cherenkov telescopes (IACTs) with a mirror diameter of 4 m, their energy threshold is 2-3 TeV.…”
Section: Introductionmentioning
confidence: 99%