TY - JOUR
T1 - SwinYNet: A Transformer-based Multitask Model for Accurate and Efficient Fast Radio Burst Searches
AU - Chen, Yunchuan
AU - Ni, Shulei
AU - Li, Chan
AU - Fang, Jianhua
AU - Zhou, Dengke
AU - Chen, Huaxi
AU - Feng, Yi
AU - Wang, Pei
AU - Jin, Chenwu
AU - Wang, Han
AU - Huang, Bijuan
AU - Guo, Xuerong
AU - Quan, Donghui
AU - Li, Di
PY - 2026/3/10
Y1 - 2026/3/10
N2 - In this study, we present a transformer-based multitask model for fast radio burst (FRB) detection, signal segmentation, and parameter estimation directly from time–frequency data, without requiring computationally expensive dedispersion preprocessing. To overcome the scarcity of labeled observational data, we develop an FRB simulator and a rule-based automatic annotation pipeline, enabling training exclusively on simulated data. Evaluations on the FAST-FREX data set show that our model achieves an F1 score of 97.8%, recall of 95.7%, and precision of 100%, outperforming both conventional tools (e.g., PRESTO, Heimdall) and recent AI-based baselines (e.g., RaSPDAM, DRAFTS) in both accuracy and inference speed. The model supports pixel-level signal segmentation and yields reliable estimates for dispersion measure and time of arrival. Large-scale blind searches on CRAFTS data further demonstrate robustness, with an average false-positive rate of 0.28% and minimal human verification required. This search has already led to the identification of two pulsar candidates, both confirmed as known pulsars. Processing benchmarks indicate that the model enables real-time searches on a single consumer-grade GPU, making petabyte-scale blind searches feasible. The code is publicly available on GitHub, and the model can be easily integrated with existing tools to automate and streamline radio data analysis beyond FRB or pulsar searches.
AB - In this study, we present a transformer-based multitask model for fast radio burst (FRB) detection, signal segmentation, and parameter estimation directly from time–frequency data, without requiring computationally expensive dedispersion preprocessing. To overcome the scarcity of labeled observational data, we develop an FRB simulator and a rule-based automatic annotation pipeline, enabling training exclusively on simulated data. Evaluations on the FAST-FREX data set show that our model achieves an F1 score of 97.8%, recall of 95.7%, and precision of 100%, outperforming both conventional tools (e.g., PRESTO, Heimdall) and recent AI-based baselines (e.g., RaSPDAM, DRAFTS) in both accuracy and inference speed. The model supports pixel-level signal segmentation and yields reliable estimates for dispersion measure and time of arrival. Large-scale blind searches on CRAFTS data further demonstrate robustness, with an average false-positive rate of 0.28% and minimal human verification required. This search has already led to the identification of two pulsar candidates, both confirmed as known pulsars. Processing benchmarks indicate that the model enables real-time searches on a single consumer-grade GPU, making petabyte-scale blind searches feasible. The code is publicly available on GitHub, and the model can be easily integrated with existing tools to automate and streamline radio data analysis beyond FRB or pulsar searches.
U2 - 10.3847/1538-4365/ae40f7
DO - 10.3847/1538-4365/ae40f7
M3 - Article
SN - 0067-0049
JO - Astrophysical Journal, Supplement Series
JF - Astrophysical Journal, Supplement Series
ER -