activity
20202026
most citedFrequency-dependent polarization of repeating fast radio bursts-implications for their origin

144 citations · 829 across the 45 of their papers we have counts for

collaborators

47 papers

astro-ph.HE2026

FAST Polarization Catalog of FRB 20240114A

Tian-Cong Wang, Jun-Shuo Zhang, Xiao-Hui Liu +60

Polarization measurements of fast radio bursts (FRBs) probe the magnetized plasma surrounding their central engines. FRB~20240114A is an exceptionally active repeating source, with…

astro-ph.HE2026★ 1 cited

The Real and Pseudo Dispersion Measures of FRB~20220912A

Yi Feng, Dengke Zhou, Y. -K. Zhang +5

Fast radio bursts (FRBs) are millisecond-duration radio transients. As they propagate through the interstellar medium, they interact with free electrons, resulting in dispersion. T…

astro-ph.HE2026

Flux Variations of Fast Radio Bursts and Their Persistent Radio Sources: Evidence for a Shared Progenitor

Xinming Li, Chenhui Niu, Jiaheng Zhang +24

Fast radio bursts (FRBs) are millisecond-duration extragalactic radio transients, some of which are associated with compact persistent radio sources (PRSs), hinting at a physical c…

astro-ph.IM2025

Towards DM-free search for Fast Radio Bursts with Machine Learning -- I. An implementation on multibeam data

Yao Chen, Rui Luo, Chen Wang +13

Searching for fleeting radio transients like fast radio bursts (FRBs) with wide-field radio telescopes has become a common challenge in data-intensive science. Conventional algorit…

astro-ph.HE2025

Identifying Quasi-Periodic Micropulses in Pulsars with FAST Using Convolutional Neural Networks

Shidong Wang, Hui Liu, Ru-Shuang Zhao +12

Quasi-periodic MicroPulses (QMP) are quasi-periodic microstructural features manifested in individual pulsar radio pulses, the study of which is crucial for understanding pulsar ra…

astro-ph.HE2025

Statistical and Temporal Analysis of Multi-component Burst-clusters from the Repeating FRB 20190520B

Jia-heng Zhang, Chen-Hui Niu, Yu-hao Zhu +10

Fast Radio Bursts (FRBs) are bright, millisecond-duration extragalactic radio transients that probe extreme astrophysical environments. Many FRBs exhibit multi-component structures…

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

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

The magnetar model's energy crisis for a prolific repeating fast radio burst source

Jun-Shuo Zhang, Tian-Cong Wang, Pei Wang +61

Fast radio bursts (FRBs) are widely considered to originate from magnetars that power the explosion through releasing magnetic energy. Active repeating FRBs have been seen to produ…

astro-ph.HE2025

Multiwavelength Observations of the Apparently Non-repeating FRB 20250316A

Ye Li, Hui Sun, Lei Qian +72

The physical origin of fast radio bursts (FRBs) remains uncertain. Although multiwavelength observations have been widely conducted, only Galactic FRB~20200428D is associated with…

astro-ph.HE2025★ 3 cited

Do Multi-Structural One-Off FRBs Trace Similar Cosmology History with Repeaters?

Yu-Hao Zhu, Chen-Hui Niu, Xiang-Han Cui +7

Fast Radio Bursts (FRBs) are millisecond-duration transient events that are typically observed at radio wavelengths and cosmological distances but their origin remains unclear. Fur…

astro-ph.HE2025★ 10 cited

Multi-year Polarimetric Monitoring of Four CHIME-Discovered Repeating Fast Radio Bursts with FAST

Yi Feng, Yong-Kun Zhang, Jintao Xie +50

In this study, we report multi-year polarization measurements of four repeating FRBs initially discovered by CHIME: FRBs~20190117A, 20190208A, 20190303A, and 20190417A. We observed…

astro-ph.HE2025★ 1 cited

Investigating FRB 20240114A with FAST: Morphological Classification and Drifting Rate Measurements in a Burst-Cluster Framework

Long-Xuan Zhang, Shiyan Tian, Junyi Shen +59

This study investigates the morphological classification and drifting rate measurement of the repeating fast radio burst (FRB) source FRB 20240114A using the Five-hundred-meter Ape…

astro-ph.HE2025★ 4 cited

A comprehensive search for Long and Short Periodic Features from an Extremely Active Cycle of FRB 20240114A

Dengke Zhou, Pei Wang, Jianhua Fang +56

Possible periodic features in fast radio bursts (FRBs) may provide insights into their astrophysical origins. Using extensive observations from the Five-hundred-meter Aperture Sphe…

astro-ph.GA2025

Why is the Star Formation Rate Proportional to Dense Gas Mass?

Sihan Jiao, Fengwei Xu, Hauyu Baobab Liu +14

One of the most profound empirical laws of star formation is the Gao-Solomon relation, a linear correlation between the star formation rate (SFR) and the dense molecular gas mass.…

astro-ph.GA2025

PANCAKE: Python bAsed Numerical Color-magnitude-diagram Analysis pacKagE

Yun Zheng, Yujiao Yang, Yong-kun Zhang +11

Stellar populations serve as a fossil record of galaxy formation and evolution, providing crucial information about the history of star formation and galaxy evolution. The color-ma…

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…

astro-ph.HE2025

The flat tail in the burst energy distribution of FRB 20240114A

Yu-Xiang Huang, Jun-Shuo Zhang, Heng Xu +19

Fast Radio Bursts (FRBs) are enigmatic millisecond-duration radio transients of extra-galactic origin, whose underlying mechanisms and progenitors remain poorly understood. FRBs ar…

astro-ph.HE2025

Polarization Position Angle Swing and the Rotating Vector Model of Repeating Fast Radio Bursts

Xiaohui Liu, Heng Xu, Jiarui Niu +23

Fast radio bursts (FRBs), typically highly polarized, usually have a nearly constant polarization position angle (PA) during each burst. Some bursts show significant PA variations,…

astro-ph.HE2025

Probing Globular Cluster with MeerKAT and FAST: A Pulsar Polarization Census

Lei Zhang, Federico Abbate, Di Li +13

Only one globular cluster (GC), 47 Tuc, has been found to contain intracluster medium, with an electron density 100 times higher than that of the ISM in its vicinity. The character…

astro-ph.GA2025

The Host Galaxy of the Hyperactive Repeating FRB 20240114A: Behind a Galaxy Cluster

Xiang-Lei Chen, Chao-Wei Tsai, Di Li +16

We report on the optical spectroscopic observations of the host galaxy of the hyperactive repeating fast radio burst, FRB 20240114A. The host galaxy is a dwarf galaxy at a redshift…

astro-ph.HE2025★ 8 cited

Hyper-active repeating fast radio bursts from rotation modulated starquakes on magnetars

Jia-Wei Luo, Jia-Rui Niu, Wei-Yang Wang +13

The non-detection of periodicity related to rotation challenges magnetar models for fast radio bursts (FRBs) with FRB emission from close to the magnetar surface. Moreover, a bimod…

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.IM2024

Accelerating FRB Search: Dataset and Methods

Xuerong Guo, Han Wang, Yifan Xiao +11

Fast Radio Burst (FRB) is an extremely energetic cosmic phenomenon of short duration. Discovered only recently and with its origin still unknown, FRBs have already started to play…