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SMILE-2+: The 2018 balloon flight and the instrument design of the electron-tracking Compton camera

机译:Smile-2 +:2018年气球航班和电子跟踪康普顿相机的仪器设计

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To establish imaging spectroscopy of cosmic gamma-rays from a few hundreds of keV to a few tens MeV, we developed an electron-tracking Compton camera (ETCC). The ETCC consists of a time projection chamber (TPC) and pixelated scintillator arrays (PSAs). The ETCC is superior to conventional gamma-ray imaging detectors of this energy band in that the arrival direction of an incident gamma-ray is firmly determined at one point and realizes high noise rejection efficiency. We performed a campaign to demonstrate the gamma-ray imaging performance of the ETCC at balloon altitude via the sub-MeV gamma-ray imaging loaded-on-balloon experiment 2+ (SMILE-2+). The balloon was launched on April 7, 2018. at 6:26 ACST (UTC +9:30) from Alice Springs, Australia. We performed a level flight for 26 hours at an altitude of 39.6 km. The main observation targets were the Galactic Center region and the Crab Nebula and we succeeded in observing them without any critical problems. The configuration of the flight, model ETCC and the housekeeping data are described in detail.
机译:要将宇宙伽马射线的成像光谱从几百kev到几千兆位建立,我们开发了一种电子跟踪康普顿相机(ETCC)。 ETCC包括时间投影室(TPC)和像素化闪烁体阵列(PSAS)。 ETCC优于该能带的传统伽马射线成像探测器,因为入射伽马射线的到达方向在一个点处牢固地确定,并实现高噪声抑制效率。我们通过亚MEV伽马射线成像加载的气球实验2+(Smile-2 +)来表现出展示ETCC的伽马射线成像性能的运动。气球于2018年4月7日推出。来自澳大利亚Alice Springs的6:26 ACST(UTC +9:30)。我们在39.6公里的海拔地区进行了26小时的水平飞行。主要观察目标是银河系中心地区和蟹星云,我们成功地观察了它们而没有任何关键问题。平飞机,模型ETCC和管家数据的配置将详细描述。

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