标题： 用于10 GeV以上伽马射线天文学的大成像空气切连科夫望远镜的蒙特卡罗研究 显示英文标题

标题： Monte Carlo Study on the Large Imaging Air Cherenkov Telescopes for >10 GeV gamma ray astronomy

摘要： 成像空气契伦科夫望远镜（IACTs），如HESS、MAGIC和VERITAS，通过在极高能伽马射线领域展示了许多令人兴奋的结果，主要在100 GeV到10 TeV之间，充分展示了它们的性能。 研究在这个能量范围内我们能够提高多少灵敏度是很重要的，但同样重要的是通过扩展这种IACT技术，将能量覆盖范围和灵敏度扩展到新的领域，即更低和更高的能量。 为此，我们通过蒙特卡罗模拟对大型IACT阵列进行了优化，假设采用新技术、先进的光电探测器和超快读出系统，特别是为了在10 GeV到100 GeV的能量范围内获得最佳灵敏度。 我们将报告具有先进技术的大型IACT阵列的性能及其局限性。 显示英文摘要

摘要： The Imaging Air Cherenkov Telescopes (IACTs), like, HESS, MAGIC and VERITAS well demonstrated their performances by showing many exciting results at very high energy gamma ray domain, mainly between 100 GeV and 10 TeV. It is important to investigate how much we can improve the sensitivity in this energy range, but it is also important to expand the energy coverage and sensitivity towards new domains, the lower and higher energies, by extending this IACT techniques. For this purpose, we have carried out the optimization of the array of large IACTs assuming with new technologies, advanced photodetectors, and Ultra Fast readout system by Monte Carlo simulation, especially to obtain the best sensitivity in the energy range between 10 GeV and 100 GeV. We will report the performance of the array of Large IACTs with advanced technologies and its limitation.