collaborators

8 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.HE2025

Sensitive Constraints on Coherent Radio Emission from Five Isolated White Dwarfs

Lei Zhang, Alexander Wolszczan, Joshua Pritchard +8

Coherent, periodic radio emission from pulsars has been widely interpreted as evidence of neutron stars as strongly magnetized compact objects. In recent years, radio pulses have a…

astro-ph.HE2025

A Target Search for Fast Radio Bursts Associated with Two Fast Blue Optical Transients: AT2018cow and CSS161010

Shi-Jie Gao, Xiang-Dong Li, Yi-Xuan Shao +5

Fast blue optical transients (FBOTs) are luminous, rapidly evolving events with blue spectra, possibly powered by newborn magnetars and linked to fast radio bursts (FRBs). Given th…

astro-ph.HE2025

Do they repeat? Monitoring 36 non-repeating FRBs with FAST

Yuri Uno, Tetsuya Hashimoto, Tomotsugu Goto +12

The origin of fast radio bursts (FRBs), highly energetic, millisecond-duration radio pulses originating from beyond our galaxy, remains unknown. Observationally, FRBs are classifie…

astro-ph.HE2025

Polarization Characteristics of the Hyperactive FRB 20240114A

Jin-Tao Xie, Yi Feng, Di Li +14

Fast radio bursts (FRBs) are transient radio bursts of extragalactic origin characterized by millisecond durations and high luminosities. We report on observations of FRB 20240114A…

astro-ph.HE2025

Bright bursts with sub-millisecond structures of FRB 20230607A in a highly magnetized environment

DeJiang Zhou, J. L. Han, Bing Zhang +19

We report the observations of a repeating FRB 20230607A for 15.6 hours spanning 16 months using the Five-hundred-meter Aperture Spherical Radio Telescope (FAST) with the detection…