Fast radio bursts: do repeaters and non-repeaters originate in statistically similar ensembles?X. H. Cui, Yiyan Yang, Changqing Ye et al.|Monthly Notices of the Royal Astronomical Society|2020Cited by 27
Evolution of Spin Period and Magnetic Field of the Crab Pulsar: Decay of the Braking Index by the Particle Wind Flow TorqueChengmin Zhang, X. H. Cui, Di Li et al.|Universe|2022Cited by 17
Luminosity distribution of fast radio bursts from CHIME/FRB Catalog 1 by means of the updated Macquart relationX. H. Cui, Yiyan Yang, Chengmin Zhang et al.|Astrophysics and Space Science|2022Cited by 15
Statistical tests of young radio pulsars with/without supernova remnants: implying two origins of neutron starsX. H. Cui, Hsiang‐Kuang Chang, Chengmin Zhang et al.|Monthly Notices of the Royal Astronomical Society|2021Cited by 9
Statistical properties of fast radio bursts elucidate their origins: magnetars are favored over gamma-ray burstsX. H. Cui, Zhen-Qi Diao, Chengmin Zhang et al.|Research in Astronomy and Astrophysics|2021Cited by 7