Differential Sensitivity of the TAIGA–IACT Facility in the Stereo Mode of Observations
摘要
Abstract
This work is devoted to the evaluation of the differential sensitivity of the 5 Imaging Atmospheric Cherenkov Telescopes (IACTs) under construction as part of the TAIGA astrophysical complex. The procedure for simulating detected gamma rays with energies from 2 to 200 TeV in the stereo mode of observations is described, along with the procedure of gamma–hadron separation for determining the differential sensitivity of the facility.