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Analysis of Commissioning Data from SST-1M : A Prototype of Single-Mirror Small Size Telescope

Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023)(2023)

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Abstract
SST-1M is a prototype of a single-mirror Small Size Telescope developed by a consortium of institutes from Poland, Switzerland and the Czech Republic. With a wide field of view of 9 degrees, SST-1Ms are designed to detect gamma-rays in the energy range between 1 and 300 TeV. The design of the SST-1M follows the Davies-Cotton concept, with a 9.42m2 multi-segment mirror. SST-1M is equipped with DigiCam camera, which features a fully digital readout and trigger system using 250 MHz ADC, and a compact Photo-Detector Plane (PDP) composed of 1296 pixels, each made of a hexagonal light guide coupled to silicone photomultipliers (SiPM). Two SST-1M telescopes are currently being commissioned at the Ondrejov Observatory in the Czech Republic, where they are successfully observing Cerenkov events in stereo. This contribution will present an overview of calibration strategies and performance evaluation based on data collected at the observatory.
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要点】:本文分析了SST-1M望远镜的调试数据,该望远镜是一种基于 Davies-Cotton 概念的单镜小型望远镜原型,能够探测1至300 TeV能量范围的伽马射线,具有创新的宽视场和数字读出系统。

方法】:文章采用了基于实际观测数据的校准策略和性能评估方法,对望远镜的各方面性能进行了详细分析。

实验】:实验在捷克共和国Ondrejov天文台的SST-1M望远镜上进行,使用了DigiCam相机和1296像素的紧凑型光电检测平面(PDP),通过收集Cerenkov事件的立体观测数据来评估望远镜性能。