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Evaluation reveals differential sensitivity of gamma-ray detection in the TAIGA astrophysical complex, indicating design effectiveness.
We evaluated the differential sensitivity of the 5 atmospheric Cherenkov telescopes under construction as part of the TAIGA astrophysical complex. The procedure of simulating of detected gamma-rays with energies from 2 to 200 TeV in the stereo observing mode is described, as well as the gamma-hadron separation technique used to determine the differential sensitivity of the facility.
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P. A. Volchugov (2025) studied this question.
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