Abstract We introduce a new simulation and analysis paradigm for Imaging Atmospheric Cherenkov Telescope (IACT) arrays, simulating the actual observation conditions as well as individual telescope configuration for each observation unit. Compared to existing frameworks, where simulations are usually generated using pre-defined settings, this run-wise simulation approach implies more realistic simulations and hence reduced systematic uncertainties. The computational effort of this dedicated simulation concept is notably independent of the amount of different observation configurations but just scales linearly with observation time. This corresponds to a large advantage for increasingly complex current and future IACT arrays where the size of the phase space makes it computationally unfeasible to generate simulations that reach the requirements regarding systematics using the classical simulation scheme.

中文翻译：

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用于成像大气切伦科夫望远镜阵列的运行智能仿真和分析框架

摘要 我们为成像大气切伦科夫望远镜 (IACT) 阵列引入了一种新的模拟和分析范式，模拟实际观测条件以及每个观测单元的单独望远镜配置。与通常使用预定义设置生成模拟的现有框架相比，这种运行方式的模拟方法意味着更真实的模拟，因此减少了系统的不确定性。这种专用模拟概念的计算工作与不同观测配置的数量无关，但仅与观测时间成线性比例。