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ELSEVIER
DOI: 10.1016/j.nima.2019.04.067
Keywords
Cosmic ray; Gamma astronomy; Timing TAIGA-HiSCORE array; Imaging TAIGA-IACT array
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Funding
- Russian Science Foundation (Section 3) [19-72-20067]
- Russian Foundation for Basic Research [18-32-00460]
- Russian Federation Ministry of Education and Science [3.9678.2017/8.9, 3.904.2017/4.6, 3.6787.2017/7.8, 3.6790.2017/7.8, 3.5917.2017/BCh]
- European Union's Horizon 2020 programme [653477]
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The combination of a wide angle timing Cherenkov array and Imaging Atmospheric Cherenkov Telescopes operated in mono mode offers a cost-effective way to construct a few square kilometers array for ultrahigh-energy gamma astronomy. The first stage of the TAIGA Observatory (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) is described here. It will comprise TAIGA-HiSCORE - 120 wide angle Cherenkov stations distributed over an area of 1.0 km(2) and three IACTs (TAIGA-IACT).
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