GRAINE 2018 experiment: Performance evaluation of gamma-ray telescope utilizing nuclear emulsion

Yuya Nakamura
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Abstract

The observation of cosmic gamma-rays is crucial to understanding high-energy astrophysical phe- nomena. The Gamma-Ray Astro-Imager with Nuclear Emulsion (GRAINE) aims to precisely ob- serve gamma-ray sources with a balloon-borne gamma-ray telescope utilizing nuclear emulsion, which is a three-dimensional tracking detector with a sub-micron spatial resolution. We launched the third balloon experiment, GRAINE 2018, on April 26, 2018 as a demonstration project. The flight was successful, data acquisition was completed, and we are analyzing the data now. We evaluated the angular resolution for gamma-rays in the 100-300 MeV energy region of the con- verter’s flight data, and it is 0.57◦ (tanθ ≃zenith angle<0.5), 0.81◦ (0.5
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GRAINE 2018实验:利用核乳剂的伽马射线望远镜性能评价
对宇宙伽马射线的观测对于理解高能天体物理现象至关重要。核乳剂伽马射线天文成像仪(GRAINE)是一种空间分辨率为亚微米的三维跟踪探测器,旨在利用核乳剂气球载伽玛射线望远镜对伽玛射线源进行精确观测。作为示范项目,我们于2018年4月26日启动了第三次气球实验——GRAINE 2018。这次飞行是成功的,数据采集已经完成,我们现在正在分析数据。我们对变换器飞行数据中100-300 MeV能量区域的伽玛射线进行了角分辨率评估,得到了0.57◦(tanθ≃天顶角<0.5)、0.81◦(0.5
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