Generating transient noise artifacts in gravitational-wave detector data with generative adversarial networks
arXiv:2207.00207 · doi:10.1088/1361-6382/acb038
Abstract
Transient noise glitches in gravitational-wave detector data limit the sensitivity of searches and contaminate detected signals. In this Paper, we show how glitches can be simulated using generative adversarial networks. We produce hundreds of synthetic images for the 22 most common types of glitches seen in the LIGO, KAGRA, and Virgo detectors. The artificial glitches can be used to improve the performance of searches and parameter-estimation algorithms. We perform a neural network classification to show that our artificial glitches are an excellent match for real glitches, with an average classification accuracy across all 22 glitch types of 99.0%.
References in corpus (12)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- Advanced LIGO
- GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
- BayesWave: Bayesian Inference for Gravitational Wave Bursts and Instrument Glitches
- Gravity Spy: Integrating Advanced LIGO Detector Characterization, Machine Learning, and Citizen Science
- LIGO Detector Characterization in the Second and Third Observing Runs
- The BayesWave analysis pipeline in the era of gravitational wave observations
- Discovering features in gravitational-wave data through detector characterization, citizen science and machine learning
- A New Method to Observe Gravitational Waves emitted by Core Collapse Supernovae
- Classification methods for noise transients in advanced gravitational-wave detectors II: performance tests on Advanced LIGO data
- On Improving the Performance of Glitch Classification for Gravitational Wave Detection by using Generative Adversarial Networks
Cited by in corpus (10)
- The Science of the Einstein Telescope
- Gravity Spy: Lessons Learned and a Path Forward
- Applications of machine learning in gravitational wave research with current interferometric detectors
- A novel stacked hybrid autoencoder for imputing LISA data gaps
- Reconstruction of binary black hole harmonics in LIGO using deep learning
- cDVGAN: One Flexible Model for Multi-class Gravitational Wave Signal and Glitch Generation
- Generative adversarial network for stellar core-collapse gravitational waves
- State Space Modelling for detecting and characterising Gravitational Waves afterglows
- Searching for topological dark matter in LIGO data
- Unveiling gravitational waves from core-collapse supernovae with MUSE