Exploring the Key Features of Repeating Fast Radio Bursts with Machine Learning

Abstract Fast radio bursts (FRBs) are enigmatic high-energy events with unknown origins, which are observationally divided into two categories, i.e., repeaters and nonrepeaters. However, there are potentially a number of nonrepeaters that may be misclassified, as repeating bursts are missed due to the limited sensitivity and observation periods, thus misleading the investigation of their physical properties. In this work, we propose a repeater identification method based on the t-distributed Stochastic Neighbor Embedding algorithm and apply the classification to the first Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst (CHIME/FRB) catalog. We find that the spectral morphology parameters, specifically spectral running ( r ), represent the key features for identifying repeaters from the nonrepeaters. Also, the results suggest that repeaters are more biased toward narrowband emission, whereas nonrepeaters are inclined toward broadband emission. We provide a list of 163 repeater candidates, five of which are confirmed with an updated repeater catalog from CHIME/FRB. Our findings improve our understanding of the various properties underlying repeaters and nonrepeaters, as well as guidelines for future FRB detection and categorization.

Authors

Publication Details

Journal
The Astrophysical Journal
Published
2025-02-13
DOI
https://doi.org/10.3847/1538-4357/adad6a
Citations
12
Primary Topic
Radio Astronomy Observations and Technology
Type
article
Field-Weighted Citation Impact
13.86

Funders

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article

Exploring the Key Features of Repeating Fast Radio Bursts with Machine Learning

Jing-Fei Zhang, Wan-Ting Hou, Wan-Peng Sun, Ji-Guo Zhang et al.
12 citations
The Astrophysical Journal
Radio Astronomy Observations and Technology
13.86
article

Exploring the Key Features of Repeating Fast Radio Bursts with Machine Learning

Jing-Fei Zhang, Wan-Ting Hou, Wan-Peng Sun, Ji-Guo Zhang, Fu-Wen Zhang, Xin Zhang, Yichao Li
article en
12 citations

Abstract

Abstract Fast radio bursts (FRBs) are enigmatic high-energy events with unknown origins, which are observationally divided into two categories, i.e., repeaters and nonrepeaters. However, there are potentially a number of nonrepeaters that may be misclassified, as repeating bursts are missed due to the limited sensitivity and observation periods, thus misleading the investigation of their physical properties. In this work, we propose a repeater identification method based on the t-distributed Stochastic Neighbor Embedding algorithm and apply the classification to the first Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst (CHIME/FRB) catalog. We find that the spectral morphology parameters, specifically spectral running ( r ), represent the key features for identifying repeaters from the nonrepeaters. Also, the results suggest that repeaters are more biased toward narrowband emission, whereas nonrepeaters are inclined toward broadband emission. We provide a list of 163 repeater candidates, five of which are confirmed with an updated repeater catalog from CHIME/FRB. Our findings improve our understanding of the various properties underlying repeaters and nonrepeaters, as well as guidelines for future FRB detection and categorization.

The Astrophysical JournalVol. 980(2)
National Natural Science Foundation of China
Openalex Percentile: Top 1%
Radio Astronomy Observations and Technology
13.86
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Exploring the Key Features of Repeating Fast Radio Bursts with Machine Learning — Jing-Fei Zhang, Wan-Ting Hou, et al. · The Astrophysical Journal (2025) | TGRS Research Map | TGRS