TAIGA—A hybrid array for high-energy gamma astronomy and cosmic-ray physics

TAIGA Collaboration, Арун Вайдянатан

Research output: Contribution to journalArticlepeer-review

5 Citations (Scopus)


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).

Original languageEnglish
Article number162113
Number of pages4
JournalNuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Publication statusPublished - 1 Apr 2020


  • Cosmic ray
  • Gamma astronomy
  • Imaging TAIGA-IACT array
  • Timing TAIGA-HiSCORE array


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