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Polarization and single-pulse micro-structure studies of Rotating Radio Transient J0139+3336 with FAST
S J Dang, J P Yuan, L H Shang, X Xu, H M Tedila, Z G Wen, W M Yan, J T Bai, Q Y Li, S Xiao, R S Zhao, Q J Zhi, A J Dong, Q D Wu, Rejep Rukiye, D D Zhang, H Yang, C B Wu and R Yuen Monthly Notices of the Royal Astronomical Society 528(2) 1213 (2024) https://doi.org/10.1093/mnras/stae046
Radio Pulsar B0950+08: Radiation in the Magnetosphere and Sparks above the Surface
The Single-pulse Observation of PSR B2111+46 with the Five-hundred-meter Aperture Spherical Radio Telescope
Q. J. Zhi, J. T. Bai, L. H. Shang, X. Xu, S. J. Dang, D. Li, L. Zhang, P. Wang, X. Y. Xie, R. S. Zhao, A. J. Dong and G. J. Qiao The Astrophysical Journal 954(1) 24 (2023) https://doi.org/10.3847/1538-4357/ace362
Strong and weak pulsar radio emission due to thunderstorms and raindrops of particles in the magnetosphere
X. Chen, Y. Yan, J. L. Han, C. Wang, P. F. Wang, W. C. Jing, K. J. Lee, B. Zhang, R. X. Xu, T. Wang, Z. L. Yang, W. Q. Su, N. N. Cai, W. Y. Wang, G. J. Qiao, J. Xu and D. J. Zhou Nature Astronomy 7(10) 1235 (2023) https://doi.org/10.1038/s41550-023-02056-z
The radio signal of PSR B0950 + 08 is detected over the whole pulse phase
Zhengli Wang, Jiguang Lu, Jinchen Jiang, et al. Monthly Notices of the Royal Astronomical Society 517(4) 5560 (2022) https://doi.org/10.1093/mnras/stac3026
Frequency Evolution Behavior of Pulse Profile of PSR B1737+13 with the Inverse Compton Scattering Model
Q. J. Zhi, X. Xu, L. H. Shang, G. J. Qiao, J. T. Bai, S. J. Dang, R. S. Zhao, A. J. Dong, D. D. Zhang, Q. W. Lin and H. Yang The Astrophysical Journal 926(1) 73 (2022) https://doi.org/10.3847/1538-4357/ac4499
A Simulation of Radius-frequency Mapping for PSR J1848-0123 with an Inverse Compton Scattering Model
L. H. Shang, X. Xu, S. J. Dang, Q. J. Zhi, J. T. Bai, R. H. Zhu, Q. W. Lin and H. Yang The Astrophysical Journal 916(2) 62 (2021) https://doi.org/10.3847/1538-4357/ac079e
How can FAST improve study of the pulsar emission mechanism and magnetospheric dynamics?
Investigating the multifrequency pulse profiles of PSRs B0329+54 and B1642–03 in an inverse Compton scattering model
Lun-Hua Shang, Ji-Guang Lu, Yuan-Jie Du, et al. Monthly Notices of the Royal Astronomical Society 468(4) 4389 (2017) https://doi.org/10.1093/mnras/stx815
MULTI-FREQUENCY RADIO PROFILES OF PSR B1133+16: RADIATION LOCATION AND PARTICLE ENERGY
J. G. Lu, Y. J. Du, L. F. Hao, Z. Yan, Z. Y. Liu, K. J. Lee, G. J. Qiao, L. H. Shang, M. Wang, R. X. Xu, Y. L. Yue and Q. J. Zhi The Astrophysical Journal 816(2) 76 (2016) https://doi.org/10.3847/0004-637X/816/2/76
MODELING THE FREQUENCY DEPENDENCE OF RADIO BEAMS FOR CONE-DOMINANT PULSARS
Turbulence, Dynamos, Accretion Disks, Pulsars and Collective Plasma Processes
G. J. Qiao, K. J. Lee, H. G. Wang and R. X. Xu Astrophysics and Space Science Proceedings, Turbulence, Dynamos, Accretion Disks, Pulsars and Collective Plasma Processes 147 (2009) https://doi.org/10.1007/978-1-4020-8868-1_10
TESTING PULSAR RADIATION MODELS USING AN α-WEAK-DEPENDENT ALTITUDE RATIO
Radio Phase-Resolved Spectra of the Conal-Double Pulsar B1133+16
Jian-Ling Chen, Hong-Guang Wang, Wan-Hai Chen, Hui Zhang and Yi Liu Chinese Journal of Astronomy and Astrophysics 7(6) 789 (2007) https://doi.org/10.1088/1009-9271/7/6/06