activity
20212026
most citedFrequency-dependent polarization of repeating fast radio bursts-implications for their origin

144 citations · 369 across the 16 of their papers we have counts for

collaborators

17 papers

astro-ph.HE2026

Constraining the Pulsar 3D Velocity Distribution: The Impact of Spin-Velocity Alignment

Zheng Li, Xiaojin Liu, Zhi-Qiang You +2

Quantifying the natal kick distribution of pulsars is essential for understanding supernova physics and binary evolution, yet measurements are historically limited by the lack of r…

astro-ph.HE2025★ 10 cited

A Persistently Active Fast Radio Burst source Embedded in an Expanding Supernova Remnant

Chen-Hui Niu, Di Li, Yuan-Pei Yang +21

Fast radio bursts (FRBs) remain one of the most puzzling astrophysical phenomena. While most FRBs are detected only once or sporadically, we present the identification of FRB 20190…

astro-ph.HE2025★ 6 cited

The double neutron star PSR J1946+2052 I. Masses and tests of general relativity

Lingqi Meng, Paulo C. C. Freire, Kevin Stovall +28

We conducted high-precision timing of PSR J1946+2052 to determine the masses of the two neutron stars in the system, test general relativity (GR) and assessed the system's potentia…

astro-ph.HE2025

Revealing the Temporally Stable Bimodal Energy Distribution of FRB 20121102A with a Tripled Burst Set from AI Detections

Yidan Wang, Jing Han, Pei Wang +34

Active repeating Fast Radio Bursts (FRBs), with their large number of bursts, burst energy distribution, and their potential energy evolution, offer critical insights into the FRBs…

astro-ph.HE2024

A 44-minute periodic radio transient in a supernova remnant

Di Li, Mao Yuan, Lin Wu +45

Long-period radio transients (LPTs) are a newly discovered class of radio emitters with periods ranging from minutes to hours. The astrophysical nature remains undetermined, partic…

astro-ph.HE2024★ 10 cited

Reinvestigation of Fast Radio Burst Host Galaxy and Event Rate Density

Wenqi Ma, Zhifu Gao, Biaopeng Li +3

Fast radio bursts (FRBs) are radio signals that last milliseconds. They originate from cosmological distances and have relatively high dispersion measures (DMs), making them being…

astro-ph.HE2024

The Variability of Persistent Radio Sources of Fast Radio Bursts

Ai Yuan Yang, Yi Feng, Chao-Wei Tsai +13

Over 700 bright millisecond-duration radio transients, known as Fast Radio Bursts (FRBs), have been identified to date. Nevertheless, the origin of FRBs remains unknown. The two re…

astro-ph.HE2024★ 8 cited

The Relativistic Spin Precession in the Compact Double Neutron Star System PSR~J1946+2052

Lingqi Meng, Weiwei Zhu, Michael Kramer +16

We observe systematic profile changes in the visible pulsar of the compact double neutron star system PSR~J1946+2052 using observations with the Five-hundred-meter Aperture Spheric…

astro-ph.HE2023★ 7 cited

Reciprocating Magnetic Fields in the Pulsar Wind Observed from the Black Widow Pulsar J1720-0534

Chen-Chen Miao, Victoria Blackmon, Wei-Wei Zhu +41

We report the radio observations of the eclipsing black widow pulsar J1720-0534, a 3.26 ms pulsar in orbit with a low mass companion of mass 0.029 to 0.034 M. We obtain t…

astro-ph.GA2023★ 9 cited

Galactic Interstellar Scintillation Observed from Four Globular Cluster Pulsars by FAST

Dandan Zhang, Zhenzhao Tao, Mao Yuan +9

We report detections of scintillation arcs for pulsars in globular clusters M5, M13 and M15 for the first time using the Five-hundred-meter Aperture Spherical radio Telescope (FAST…

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.HE2023★ 24 cited

The arrival time and energy of FRBs traverse the time-energy bivariate space like a Brownian motion

Yong-Kun Zhang, Di Li, Yi Feng +5

The origin of fast radio bursts (FRBs), the brightest cosmic explosion in radio bands, remains unknown. We introduce here a novel method for a comprehensive analysis of active FRBs…

astro-ph.HE2022★ 82 cited

FAST observations of an extremely active episode of FRB 20201124A: II. Energy Distribution

Yong-Kun Zhang, Pei Wang, Yi Feng +17

We report the properties of more than 800 bursts detected from the repeating fast radio burst (FRB) source FRB 20201124A with the Five-hundred-meter Aperture Spherical radio Telesc…

astro-ph.HE2022★ 15 cited

Interstellar scintillation and polarization of PSR B0656+14 in the Monogem Ring

Jumei Yao, William A. Coles, Richard N. Manchester +8

High sensitivity interstellar scintillation and polarization observations of PSR~B0656+14 made at three epochs over a year using the Five-hundred-meter Aperture Spherical radio Tel…

astro-ph.HE2022★ 144 cited

Frequency-dependent polarization of repeating fast radio bursts-implications for their origin

Yi Feng, Di Li, Yuan-Pei Yang +23

The polarization of fast radio bursts (FRBs), bright astronomical transients, contains crucial information about their environments. We report polarization measurements of five rep…

astro-ph.HE2021★ 41 cited

FAST discovery of an extremely radio-faint millisecond pulsar from the Fermi-LAT unassociated source 3FGL J0318.1+0252

Pei Wang, Di Li, Colin J. Clark +23

High sensitivity radio searches of unassociated -ray sources have proven to be an effective way of finding new pulsars. Using the Five-hundred-meter Aperture Spherical radio Tel…

astro-ph.GA2021★ 4 cited

The first evidence for three-dimensional spin-velocity alignment in pulsars

Jumei Yao, Weiwei Zhu, Richard N. Manchester +11

More than 50 years after the discovery of pulsars and confirmation of their association with supernova explosions, the origin of the initial spin and velocity of pulsars remains la…