English

Attention U-Net for all-sky continuous gravitational wave searches

General Relativity and Quantum Cosmology 2025-09-29 v2 Instrumentation and Methods for Astrophysics Instrumentation and Detectors

Abstract

Detecting continuous gravitational waves is challenging due to the high computational cost of template-based searches across large parameter spaces, particularly for all-sky searches. Machine learning offers a promising solution to perform these searches with reasonable computational resources. In this study, we trained an attention U-Net, a convolutional neural network, on \approx 10.67 days of simulated data with Gaussian noise for all-sky searches at different frequencies within the 20-1000 Hz band. Our model trained at 20 Hz achieves the best sensitivity, with a 90% detection efficiency sensitivity depth D90%=29.97±0.24Hz1/2D^{90\%} = 29.97 \pm 0.24\,\mathrm{Hz}^{-1/2} with a 1% false alarm rate per 50 mHz, while the model trained on the entire 20-1000 Hz band yields D90%=18.63±0.24Hz1/2D^{90\%} = 18.63 \pm 0.24\,\mathrm{Hz}^{-1/2}. The sensitivities achieved are comparable to state-of-the-art results using deep learning approaches, with less than 50% of the training time and data. We find that sensitivity scales as T0.28±0.01T^{0.28 \pm 0.01} with total observation time for the attention U-Net trained at 20 Hz, similar to semi-coherent search methods. The neural network demonstrates robustness on datasets with time gaps, with sensitivity dependence on duty factor analyzed. We also investigated the sensitivity dependence of the trained attention U-Net models on sky location. Our findings show that attention U-Net is a scalable and effective approach for all-sky continuous gravitational wave searches.

Keywords

Cite

@article{arxiv.2509.19838,
  title  = {Attention U-Net for all-sky continuous gravitational wave searches},
  author = {Damon H. T. Cheung},
  journal= {arXiv preprint arXiv:2509.19838},
  year   = {2025}
}

Comments

10 pages, 7 figures