activity
20192025
most citedPSR J1926-0652: A Pulsar with Interesting Emission Properties Discovered at FAST

45 citations · 303 across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.HE2025

The diverse morphology of gravitational wave signals from merging neutron-star white-dwarf binaries

Shenghua Yu, Youjun Lu, C. Simon Jeffery +6

In sufficiently compact neutron star-white dwarf (NSWD) binary systems, orbital decay means the white dwarf eventually fills its shrinking Roche lobe, initiating a phase of mass tr…

astro-ph.HE2025

Detecting FRB by DANCE: a method based on DEnsity ANalysis and Cluster Extraction

Mao Yuan, Jiarui Niu, Yi Feng +7

Fast radio bursts (FRBs) are transient signals exhibiting diverse strengths and emission bandwidths. Traditional single-pulse search techniques are widely employed for FRB detectio…

astro-ph.HE2023★ 9 cited

High-altitude Magnetospheric Emissions from Two Pulsars

Mao Yuan, Weiwei Zhu, Michael Kramer +21

We discover three new weak pulse components in two known pulsars, one in PSR J0304+1932 and two in PSR J1518+4904. These components are emitted about half way between the main emis…

astro-ph.HE2022★ 18 cited

Evolution of Spin Period and Magnetic Field of the Crab Pulsar: Decay of the Braking Index by the Particle Wind Flow Torque

Cheng-Min Zhang, Xiang-Han Cui, Di Li +8

The evolutions of a neutron star's rotation and magnetic field (B-field) have remained unsolved puzzles for over half a century. We ascribe the rotational braking torques of pulsar…

astro-ph.HE2022★ 16 cited

Luminosity distribution of fast radio bursts from CHIME/FRB Catalog 1 by means of the updated Macquart relation

Xiang-Han Cui, Cheng-Min Zhang, Di Li +9

Fast radio bursts (FRBs) are extremely strong radio flares lasting several micro- to milliseconds and come from unidentified objects at cosmological distances, most of which are on…

astro-ph.IM2022★ 9 cited

Categorize Radio Interference using component and temporal analysis

Mao Yuan, Weiwei Zhu, Haiyan Zhang +12

Radio frequency interference (RFI) is a significant challenge faced by today's radio astronomers. While most past efforts were devoted to cleaning the RFI from the data, we develop…