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CAS IR Grid
机构
国家授时中心 [2]
国家空间科学中心 [1]
光电技术研究所 [1]
高能物理研究所 [1]
合肥物质科学研究院 [1]
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OAI收割 [6]
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期刊论文 [6]
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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
single-pixel imaging
binary modulation
multi-object positioning
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
data rate
enhanced Loran (eLoran) system
extended binary phase shift keying (EBPSK) modulation
ultra narrow band (UNB) modulation
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
Compressive imaging
Discrete cosine transform
Single-pixel
Binary modulation
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
PARAMETRIC DOWNCONVERSION
2-PHOTON ABSORPTION
AXIAL RESOLUTION
GENERATION
ULTRABROADBAND
FLUORESCENCE
ENTANGLEMENT
ENERGY
LIGHT
chirped biphotons
correlation times
compression
binary phase modulation
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
Super-oscillatory Lens
Cylindrical-vector Beams
Long Focal Length
Phase Modulation
Far-field
Light
Amplitude
Binary
Spot
Superresolution