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Insight-HXMT study of the timing properties of Sco X-1 期刊论文
2021, 卷号: 43, 页码: 1613
作者:  Jia, Shumei
收藏  |  浏览/下载：24/0  |  提交时间：2021/11/18
The observational properties of black hole X-ray binary transients by insight-HXMT 期刊论文
2021, 卷号: 43, 页码: 1587p.1587
作者:  Qu, Jinlu;  Huang, Yue;  Liu, Hexin
收藏  |  浏览/下载：31/0  |  提交时间：2021/11/18
Time-lag Between Disk and Corona Radiation Leads to Hysteresis Effect Observed in Black hole X-Ray Binary MAXI J1348-630 期刊论文
The Astrophysical Journal, 2021, 卷号: 915, 页码: L15
作者:  Weng, Shan-Shan;  Cai, Zhen-Yi;  Zhang, Shuang-Nan;  Zhang, Wei;  Chen, Yu-Peng
收藏  |  浏览/下载：11/0  |  提交时间：2021/11/18
Modeling multiband X-ray light curves of the Crab pulsar with the annular and core gap models 期刊论文
New Astronomy, 2021, 卷号: 83, 页码: 101480
作者:  Jun-Tao, Bai;  Xin, Xu;  Quan-Wei, Lin;  Qi-Jun, Zhi;  Lun-Hua, Shang
收藏  |  浏览/下载：43/0  |  提交时间：2021/11/18
Insight-HXMT study of the timing properties of Sco X-1 期刊论文
Journal of High Energy Astrophysics, 2020, 卷号: 25, 页码: 1-9
作者:  The Insight-HXMT Collaboration
收藏  |  浏览/下载：2/0  |  提交时间：2020/03/27
Detection of high flux synchrotron radiation based on diamond detector for heps 期刊论文
Nuclear instruments & methods in physics research section a-accelerators spectrometers detectors and associated equipment, 2019, 卷号: 924, 页码: 305-308
作者:  Li Zhenjie;  Wang Bingjie;  Chang Guangcai;  Li Qiuju;  Zhou Yangfan
收藏  |  浏览/下载：94/0  |  提交时间：2019/04/22
Detection of high flux synchrotron radiation based on diamond detector for heps 期刊论文
Nuclear instruments & methods in physics research section a-accelerators spectrometers detectors and associated equipment, 2019, 卷号: 924, 页码: 305-308
作者:  Li Zhenjie;  Wang Bingjie;  Chang Guangcai;  Li Qiuju;  Zhou Yangfan
收藏  |  浏览/下载：94/0  |  提交时间：2019/04/22
Search for gamma-ray emission from the sun during solar minimum with the argo-ybj experiment 期刊论文
The astrophysical journal, 2019, 卷号: 872, 期号: 2
作者:  Bartoli,B.;  Bernardini,P.;  Bi,X. J.;  Cao,Z.;  Catalanotti,S.
收藏  |  浏览/下载：127/0  |  提交时间：2019/04/23
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.  
Investigation of the multiplet features of srtio3 in x-ray absorption spectra based on configuration interaction calculations 期刊论文
Journal of synchrotron radiation, 2018, 卷号: 25, 页码: 777-784
作者:  Wu, M.;  Xin, Houlin L.;  Wang, J. O.;  Li, X. J.;  Yuan, X. B.
收藏  |  浏览/下载：29/0  |  提交时间：2019/04/23

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