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Multi-Object Positioning and Imaging Based on Single-Pixel Imaging Using Binary Patterns 期刊论文  OAI收割
SENSORS, 2022, 卷号: 22
作者:  
Meng, Wenwen;  Shi, Dongfeng;  Yang, Wei;  Zha, Linbin;  Zhao, Yuefeng
  |  收藏  |  浏览/下载:39/0  |  提交时间:2022/12/23
Application of Ultra Narrow Band Modulation in Enhanced Loran System 期刊论文  OAI收割
SENSORS, 2021, 卷号: 21, 期号: 13, 页码: 12
作者:  
Lyu, Boyun;  Hua, Yu;  Yuan, Jiangbin;  Li, Shifeng
  |  收藏  |  浏览/下载:31/0  |  提交时间:2021/11/29
Discrete cosine single-pixel microscopic compressive imaging via fast binary modulation 期刊论文  OAI收割
OPTICS COMMUNICATIONS, 2020, 卷号: 454, 页码: UNSP 124512
作者:  
Chen, Ying;  Liu, Shuai;  Yao, Xu-Ri;  Zhao, Qing;  Liu, Xue-Feng
  |  收藏  |  浏览/下载:339/0  |  提交时间:2019/12/17
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:56/0  |  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.  
Compression of correlation time of chirped biphotons by binary phase modulation 期刊论文  OAI收割
ACTA PHYSICA SINICA, 2017, 卷号: 66, 期号: 4
作者:  
Li BH(李百宏);  Wang DD(王豆豆);  Pang HF(庞华锋);  Zhang T(张涛);  Jie Y(解忧)
  |  收藏  |  浏览/下载:8/0  |  提交时间:2021/01/11
Generation of a sub-diffraction hollow ring by shaping an azimuthally polarized wave 期刊论文  OAI收割
SCIENTIFIC REPORTS, 2016, 卷号: 6
作者:  
Chen, Gang;  Wu, Zhi-Xiang;  Yu, An-ping;  Zhang, Zhi-hai;  Wen, Zhong-quan
  |  收藏  |  浏览/下载:42/0  |  提交时间:2018/06/14