4.2 Article

In-flight calibration of the Insight-Hard X-ray Modulation Telescope

期刊

JOURNAL OF HIGH ENERGY ASTROPHYSICS
卷 27, 期 -, 页码 64-76

出版社

ELSEVIER
DOI: 10.1016/j.jheap.2020.02.009

关键词

X-ray instrument; Insight-HXMT; Calibration

资金

  1. National Natural Science Foundation of China [U1838105, U1838201, U1838202]
  2. National Program on Key Research and Development Project [2016YFA0400800]
  3. China National Space Administration (CNSA)
  4. Chinese Academy of Sciences (CAS)

向作者/读者索取更多资源

We present the calibration of the Insight-Hard X-ray Modulation Telescope(Insight-HXMT) X-ray satellite, which can be used to perform timing and spectral studies of bright X-ray sources. Insight-HXMTcarries three main payloads onboard: the High Energy X-ray telescope (HE), the Medium Energy X-ray telescope (ME) and the low Energy X-ray telescope (LE). In orbit, the radioactive sources, activated lines, the fluorescence lines and celestial sources are used to calibrate the energy scale and energy resolution of the payloads. The Crab nebular is adopted as the primary effective area calibrator and empirical functions are constructed to modify the simulated effective areas of the three payloads respectively. The systematic errors of HE, compared to the model of the Crab nebular, are less than 2% in 28-120keV and 2%-10% above 120keV. The systematic errors of ME are less than 1.5% in 10-35keV. The systematic errors of LE are less than 1% in 1-7keV except the Si K-edge (1.839keV, up to 1.5%) and less than 2% in 7-10keV. (C) 2020 Elsevier B.V. All rights reserved.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.2
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据