Denoising Gravitational Waves with Enhanced Deep Recurrent Denoising Auto-Encoders
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Abstract (arXiv)
Denoising of time domain data is a crucial task for many applications such as communication, translation, virtual assistants etc. For this task, a combination of a recurrent neural net (RNNs) with a Denoising Auto-Encoder (DAEs) has shown promising results. However, this combined model is challenged when operating with low signal-to-noise ratio (SNR) data embedded in non-Gaussian and non-stationary noise. To address this issue, we design a novel model, referred to as 'Enhanced Deep Recurrent Denoising Auto-Encoder' (EDRDAE), that incorporates a signal amplifier layer, and applies curriculum learning by first denoising high SNR signals, before gradually decreasing the SNR until the signals become noise dominated. We showcase the performance of EDRDAE using time-series data that describes gravitational waves embedded in very noisy backgrounds. In addition, we show that EDRDAE can accurately denoise signals whose topology is significantly more complex than those used for training, demonstrating that our model generalizes to new classes of gravitational waves that are beyond the scope of established denoising algorithms.
Key facts. Cited by 10 papers in the map (data through 14 Oct 2026). First posted on arXiv 6 Mar 2019.
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Citing papers per year: 2021: 3; 2022: 5; 2023: 0; 2024: 1; 2025: 1.
10 papers.
- 2022Astronomia ex machina: a history, primer, and outlook on neural networks in astronomycited by 17
- 2021Advances in Machine and Deep Learning for Modeling and Real-time Detection of Multi-Messenger Sourcescited by 10
- 2021Interpretable AI forecasting for numerical relativity waveforms of quasi-circular, spinning, non-precessing binary black hole mergerscited by 5
- 2022Inference-optimized AI and high performance computing for gravitational wave detection at scalecited by 5
- 2021AI and extreme scale computing to learn and infer the physics of higher order gravitational wave modes of quasi-circular, spinning, non-precessing binary black hole mergerscited by 3
- 2022Boosting the Efficiency of Parametric Detection with Hierarchical Neural Networkscited by 1
- 2025DeepExtractor: Time-domain reconstruction of signals and glitches in gravitational wave data with deep learningcited by 1
- 2022Data-driven detector signal characterization with constrained bottleneck autoencoderscited by 0
- 2022DeepSNR: A deep learning foundation for offline gravitational wave detectioncited by 0
- 2024Transfer Learning Adapts to Changing PSD in Gravitational Wave Datacited by 0
- 2025DeepExtractor: Time-domain reconstruction of signals and glitches in gravitational wave data with deep learning30 Jan 2025
- 2024Transfer Learning Adapts to Changing PSD in Gravitational Wave Data15 Oct 2024
- 2022Astronomia ex machina: a history, primer, and outlook on neural networks in astronomy7 Nov 2022
- 2022Boosting the Efficiency of Parametric Detection with Hierarchical Neural Networks23 Jul 2022
- 2022DeepSNR: A deep learning foundation for offline gravitational wave detection11 Jul 2022
- 2022Data-driven detector signal characterization with constrained bottleneck autoencoders9 Mar 2022
- 2022Inference-optimized AI and high performance computing for gravitational wave detection at scale26 Jan 2022
- 2021AI and extreme scale computing to learn and infer the physics of higher order gravitational wave modes of quasi-circular, spinning, non-precessing binary black hole mergers13 Dec 2021
- 2021Interpretable AI forecasting for numerical relativity waveforms of quasi-circular, spinning, non-precessing binary black hole mergers13 Oct 2021
- 2021Advances in Machine and Deep Learning for Modeling and Real-time Detection of Multi-Messenger Sources13 May 2021