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The High Energy X-ray telescope (HE) onboard the Insight-HXMT astronomy satellite 期刊论文
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2020, 卷号: 63, 期号: 4, 页码: 249503
作者:  Liu, CongZhan;  Zhang, YiFei;  Li, XuFang;  Lu, XueFeng;  Chang, Zhi
收藏  |  浏览/下载：35/0  |  提交时间：2020/10/19
Comparison of simulated backgrounds with in-orbit observations for HE, ME, and LE onboard Insight-HXMT 期刊论文
Astrophysics and Space Science, 2020, 卷号: 365, 页码: 158
作者:  HXMT
收藏  |  浏览/下载：19/0  |  提交时间：2022/02/08
HXMT卫星空间环境监测器及初步观测结果 期刊论文
空间科学学报, 2019, 卷号: 39, 期号: 6, 页码: 770-777
作者:  王春琴;  沈国红;  张珅毅;  常峥;  袁斌
收藏  |  浏览/下载：2/0  |  提交时间：2020/03/12
X射线脉冲星动态信号处理方法研究 期刊论文
深空探测学报, 2019, 卷号: 6, 期号: 04, 页码: 335-340
作者:  张大鹏;  李治泽;  王奕迪;  郑伟
收藏  |  浏览/下载：2/0  |  提交时间：2020/03/27
Constant cyclotron line energy in Hercules X-1 - Joint Insight-HXMT and NuSTAR observations 期刊论文
Journal of High Energy Astrophysics, 2019, 卷号: 23, 页码: 29-32
作者:  HXMT
收藏  |  浏览/下载：33/0  |  提交时间：2022/02/08
Timing analysis of Swift J1658.2-4242's outburst in 2018 with Insight-HXMT, NICER and AstroSat 期刊论文
Journal of High Energy Astrophysics, 2019, 卷号: 24, 页码: 30-40
作者:  HXMT
收藏  |  浏览/下载：41/0  |  提交时间：2022/02/08
Accretion  accretion disks  Black hole physics  X-rays: binaries:  Swift J1658.2-4242  Astrophysics - High Energy Astrophysical Phenomena  Abstract: We present the observational results from a detailed timing analysis of the black hole candidate Swift J1658.2-4242 during its 2018 outburst with the observations of Hard X-ray Modulation Telescope (Insight-HXMT), Neutron Star Interior Composition Explorer (NICER) and AstroSat in 0.1-250 keV. The evolution of intensity, hardness and integrated fractional root mean square (rms) observed by Insight-HXMT and NICER are presented in this paper. Type-C quasi-periodic oscillations (QPOs) observed by NICER (0.8-3.5 Hz) and Insight-HXMT (1-1.6 Hz) are also reported in this work. The features of the QPOs are analyzed with an energy range of 0.5-50 keV. The relations between QPO frequency and other characteristics such as intensity, hardness and QPO rms are carefully studied. The timing and spectral properties indicate that Swift J1658.2-4242 is a black hole binary system. Besides, the rms spectra of the source calculated from the simultaneous observation of Insight-HXMT, NICER and AstroSat support the Lense-Thirring origin of the QPOs. The relation between QPO phase lag and the centroid frequency of Swift J1658.2-4242 reveals a near zero constant when < 4Hz and a soft phase lag at 6.68 Hz. This independence follows the same trend as the high inclination galactic black hole binaries such as MAXI J1659-152.  
Ground-based calibration and characterization of the HE detectors for Insight-HXMT 期刊论文
Journal of High Energy Astrophysics, 2019, 卷号: 24, 页码: 6-14
作者:  HXMT
收藏  |  浏览/下载：10/0  |  提交时间：2022/02/08
Insight-HXMT science operations 期刊论文
2018, 页码: 10704
作者:  Qu, J. L;  Zhang, S.;  Chen, L.  ;  Jia, S. M;  Ma, X
收藏  |  浏览/下载：7/0  |  提交时间：2019/07/11

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