Enomoto, RHara, ShinjiAsahara, ABicknell, GeoffreyEdwards, Philip GGunji, SHara, TJimbo, J.Kajino, FKatagiri, HKataoka, JKawachi, AKifune, TadashiKubo, HKushida, JMatsubara, YMizumoto, YMori, MasakiMoriya, MieMuraishi, HMuraki, YNaito, TNakase, TNishijima, KOkumura, KPatterson, Joseph RSakurazawa, KSwaby, D LTakano, KTanimori, TTamura, TTsuchiya, KUruma, KYanagita, SYoshida, TYoshikoshi, TYuki, A2015-12-100927-6505http://hdl.handle.net/1885/68586CANGAROO-III is an imaging atmospheric Cherenkov telescope array of four 10-m telescopes for very high energy (sub-TeV) γ-ray astronomy. A design study of the CANGAROO-III telescope system was carried out using the Monte Carlo technique in order to optimKeywords: Astronomy; Diamonds; Gamma rays; Imaging techniques; Optimization; Particle detectors; Cherenkov telescopes; Energy threshold; Threshold energy; Zenith angle; Space telescopes200210.1016/S0927-6505(01)00112-82015-12-10