collaborators

6 papers

astro-ph.HE2026

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.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.HE2026

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

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.HE2025

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…