Detecting FRB by DANCE: a method based on DEnsity ANalysis and Cluster Extraction

ABSTRACT Fast radio bursts (FRBs) are transient signals exhibiting diverse strengths and emission bandwidths. Traditional single-pulse search techniques are widely employed for FRB detection; yet weak, narrow-band bursts often remain undetectable due to low signal-to-noise ratios (SNR) in integrated profiles. We developed DANCE, a detection tool based on cluster analysis of the original spectrum. It is specifically designed to detect and isolate weak, narrow-band FRBs, providing direct visual identification of their emission properties. This method performs density clustering on reconstructed, RFI-cleaned observational data, enabling the extraction of targeted clusters in time-frequency domain that correspond to the genuine FRB emission range. Our simulations show that DANCE successfully extracts all true signals with SNR $>5$ and achieves a detection precision exceeding 93 per cent. Furthermore, through the practical detection of FRB 20201124A, DANCE has demonstrated a significant advantage in finding previously undetectable weak bursts, particularly those with distinct narrow-band features or occurring in proximity to stronger bursts.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2025-11-06
DOI
https://doi.org/10.1093/mnras/staf1910
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
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article

Detecting FRB by DANCE: a method based on DEnsity ANalysis and Cluster Extraction

Jiarui Niu, Jingye Yan, Mao Yuan, Yi Feng et al.
Monthly Notices of the Royal Astronomical Society
Pulsars and Gravitational Waves Research
article

Detecting FRB by DANCE: a method based on DEnsity ANalysis and Cluster Extraction

Jiarui Niu, Jingye Yan, Mao Yuan, Yi Feng, Weiwei Zhu, Lingqi Meng, Li Deng, Bo Peng, Chenchen Miao, Xiaoyin Lv
article en

Abstract

ABSTRACT Fast radio bursts (FRBs) are transient signals exhibiting diverse strengths and emission bandwidths. Traditional single-pulse search techniques are widely employed for FRB detection; yet weak, narrow-band bursts often remain undetectable due to low signal-to-noise ratios (SNR) in integrated profiles. We developed DANCE, a detection tool based on cluster analysis of the original spectrum. It is specifically designed to detect and isolate weak, narrow-band FRBs, providing direct visual identification of their emission properties. This method performs density clustering on reconstructed, RFI-cleaned observational data, enabling the extraction of targeted clusters in time-frequency domain that correspond to the genuine FRB emission range. Our simulations show that DANCE successfully extracts all true signals with SNR $>5$ and achieves a detection precision exceeding 93 per cent. Furthermore, through the practical detection of FRB 20201124A, DANCE has demonstrated a significant advantage in finding previously undetectable weak bursts, particularly those with distinct narrow-band features or occurring in proximity to stronger bursts.

Monthly Notices of the Royal Astronomical SocietyVol. 544(4)
Chinese Academy of Sciences (CN), Beijing Normal University (CN), Chengdu Institute of Information Technology (China) (CN), Qilu Normal University (CN), National Space Science Center (CN), Zhejiang Lab (CN), National Astronomical Observatories (CN)
Openalex Percentile: Top 77%
Pulsars and Gravitational Waves Research
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