天空
有效载荷(计算)
伽马射线暴
闪烁体
卫星
物理
船上
伽马射线
航程(航空)
遥感
探测器
光学
天体物理学
天文
航空航天工程
计算机科学
工程类
地质学
网络数据包
计算机网络
作者
Hsiang‐Kuang Chang,Chi-Hsun Lin,Che-Chih Tsao,Che-Yen Chu,Shun-Chia Yang,Chien-You Huang,Chao-Hsi Wang,Tze-Hsiang Su,Yun-Hsin Chung,Y. H. Chang,Zijun Gong,Jr-Yue Hsiang,Keng-Li Lai,Tsu-Hsuan Lin,Chia-Yü Lu,Chien-Ying Yang
标识
DOI:10.1016/j.asr.2021.10.044
摘要
The Gamma-ray Transients Monitor (GTM) is a secondary payload on board Formosat-8B (FS-8B), a Taiwanese remote-sensing satellite scheduled to launch in 2024. The goal of GTM is to monitor Gamma Ray Bursts (GRBs) and other bright gamma-ray transients in the energy range from 50 keV to 2 MeV. GTM consists of two identical modules located on two opposite sides of FS-8B. Each module has four sensor units facing different directions to cover half of the sky. The two modules will then cover the whole sky, including the direction occulted by the Earth. Each sensor unit is composed of a GAGG scintillator array (50 mm × 50 mm × 8 mm) to be readout by SiPM with 16 pixel-channels. We describe the instrument design and its GRB detection efficiency in this paper. GTM is expected to detect about 40 GRBs per year.
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