TAIGA array addresses gamma-ray astronomy at energies from a few TeV to several PeV as well as cosmic ray physics from 100 TeV to several EeV. A 1 km2 TAIGA setup will consist of 120 wide-Angle detectors of the Cherenkov timing array TAIGA-HiSCORE and three imaging air Cherenkov telescopes with the field of view diameter of 9.6°. In this paper, first experimental results of the first operation stage are presented: signal detection from two gamma-ray sources, the Crab Nebula and Markarian 421, by the first IACT in stand-Alone mode. The detected signal is shown to be in agreement with the Monte Carlo expectation. In future, gamma-ray signal will be detected by a larger number of TAIGA telescopes as well as the TAIGA-HiSCORE array, that is, in combined operation mode.
|Журнал||Journal of Physics: Conference Series|
|Состояние||Опубликовано - 16 дек 2020|
|Событие||5th International Conference on Particle Physics and Astrophysics, ICPPA 2020 - Moscow, Virtual, Российская Федерация|
Продолжительность: 5 окт 2020 → 9 окт 2020