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浏览/检索结果: 共6条,第1-6条 帮助

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Frequency steering of spaceborne clocks based on XPNAV-1 observations 期刊论文  OAI收割
CHINESE JOURNAL OF AERONAUTICS, 2023, 卷号: 36, 期号: 6, 页码: 266-278
作者:  
Han, Mengna;  Tong, Minglei;  LI, Liansheng;  Shi, Yongqiang;  Yang, Tinggao
  |  收藏  |  浏览/下载:37/0  |  提交时间:2023/12/13
Real-time monitoring of the dynamic variation of satellite orbital maneuvers based on BDS observations 期刊论文  OAI收割
MEASUREMENT, 2021, 卷号: 168, 页码: 9
作者:  
Tu, Rui;  Zhang, Rui;  Fan, Lihong;  Han, Junqiang;  Zhang, Pengfei
  |  收藏  |  浏览/下载:25/0  |  提交时间:2021/11/29
Real-time detection of BDS orbit manoeuvres based on the combination of GPS and BDS observations 期刊论文  OAI收割
IET RADAR SONAR AND NAVIGATION, 2020, 卷号: 14, 期号: 10, 页码: 1603-1609
作者:  
Tu, Rui;  Zhang, Rui;  Liu, Zhanke;  Fan, Lihong;  Han, Junqiang
  |  收藏  |  浏览/下载:40/0  |  提交时间:2021/11/29
Timing analysis of Swift J1658.2-4242's outburst in 2018 with Insight-HXMT, NICER and AstroSat 期刊论文  OAI收割
Journal of High Energy Astrophysics, 2019, 卷号: 24, 页码: 30-40
作者:  
HXMT
  |  收藏  |  浏览/下载:61/0  |  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.  
Design of a CDS ASIC for Multireadout X-Ray CCDs With a 0.032% INL 期刊论文  OAI收割
IEEE TRANSACTIONS ON NUCLEAR SCIENCE, 2018, 卷号: 65, 期号: 6, 页码: 1307-1314
作者:  
Lu B(陆波);  Lu, B;  Chen, Y;  Chen Y(陈勇)
  |  收藏  |  浏览/下载:45/0  |  提交时间:2019/09/24
Observational features of pulsar glitches 期刊论文  OAI收割
Science China Physics,Mechanics & Astonomy, 2010, 卷号: 53, 期号: 增刊1, 页码: 3-8
作者:  
WANG Na;  YUAN JianPing
收藏  |  浏览/下载:16/0  |  提交时间:2013/03/06
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