Details

Autor(en) / Beteiligte

• Liu, CongZhan
• Zhang, YiFei
• Li, XuFang
• Lu, XueFeng
• Chang, Zhi
• Li, ZhengWei
• Zhang, AiMei
• Jin, YongJie
• Yu, HuiMing
• Zhang, Zhao
• Fu, MinXue
• Chen, YiBao
• Ji, JianFeng
• Xu, YuPeng
• Deng, JingKang
• Shang, RenCheng
• Liu, GuoQing
• Lu, FangJun
• Zhang, ShuangNan
• Dong, YongWei
• Li, TiPei
• Wu, Mei
• Li, YanGuo
• Wang, HuanYu
• Wu, BoBing
• Zhang, YongJie
• Zhang, Zhi
• Xiong, ShaoLin
• Liu, Yuan
• Zhang, Shu
• Liu, HongWei
• Yang, YiJung
• Zhang, Fan

Titel

The High Energy X-ray telescope (HE) onboard the Insight-HXMT astronomy satellite

Ist Teil von

• Science China. Physics, mechanics & astronomy, 2020-04, Vol.63 (4), p.249503, Article 249503

Ort / Verlag

Beijing: Science China Press

Erscheinungsjahr

2020

Link zum Volltext

Quelle

Alma/SFX Local Collection

Beschreibungen/Notizen

• The Insight -Hard X-ray Modulation Telescope ( Insight -HXMT) is a broadband X-ray and γ-ray (1-3000 keV) astronomy satellite. One of its three main telescopes is the High Energy X-ray telescope (HE). The main detector plane of HE comprises 18 NaI(Tl)/CsI(Na) phoswich detectors, where NaI(Tl) is used as the primary detector to measure ~ 20–250 keV photons incident from the field of view (FOV) defined by collimators, and CsI(Na) is used as the active shielding detector to NaI(Tl) by pulse shape discrimination. Additionally, CsI(Na) is used as an omnidirectional γ-ray monitor. The HE collimators have a diverse FOV, i.e. 1.1°×5.7° (15 units), 5.7°×5.7° (2 units), and blocked (1 unit). Therefore, the combined FOV of HE is approximately 5.7°×5.7°. Each HE detector has a diameter of 190 mm resulting in a total geometrical area of approximately 5100 cm 2 , and the energy resolution is ~15% at 60 keV. For each recorded X-ray event by HE, the timing accuracy is less than 10 μs and the dead-time is less than 10 μs. HE is used for observing spectra and temporal variability of X-ray sources in the 20–250 keV band either by pointing observations for known sources or scanning observations to unveil new sources. Additionally, HE is used for monitoring the γ-ray burst in 0.2-3 MeV band. This paper not only presents the design and performance of HE instruments but also reports results of the on-ground calibration experiments.