학술논문

Tunka Advanced Instrument for cosmic rays and Gamma Astronomy (TAIGA): Status, results and perspectives.
Document Type
Article
Source
EPJ Web of Conferences. 2017, Vol. 145, p1-8. 8p.
Subject
*COSMIC rays
*ASTROPHYSICS
*DETECTORS
*MUONS
*CHERENKOV counters
*SOCIETIES
Language
ISSN
2101-6275
Abstract
We present the current status of high-energy cosmic-ray physics and gamma-ray astronomy at the Tunka Astrophysical Center (AC). This complex is located in the Tunka Valley, about 50 km from Lake Baikal. Present efforts are focused on the construction of the first stage of the gamma-ray observatory TAIGA - the TAIGA prototype. TAIGA (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) is designed for the study of gamma rays and charged cosmic rays in the energy range 1013 eV-1018 eV. The array includes a network of wide angle timing Cherenkov stations (TAIGA-HiSCORE), each with a FOV= 0.6 sr, plus up to 16 IACTs (FOV - 10° × 10°). This part covers an area of 5 km2. Additional muon detectors (TAIGAMuon), with a total coverage of 2000m2, are distributed over an area of 1 km2. [ABSTRACT FROM AUTHOR]