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Simulating Transient Noise Bursts in LIGO with gengli

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arxiv 2205.09204 v2 pith:HMVPB6IM submitted 2022-05-18 astro-ph.IM

classification astro-ph.IM
keywords glitchestransientdetectiongenglinetworknoiseadversarialamount
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abstract

In the field of gravitational-wave (GW) interferometers, the most severe limitation to the detection of transient signals from astrophysical sources comes from transient noise artefacts, known as glitches, that happens at a rate around $1$ per minute. Because glitches reduce the amount of scientific data available, there is a need for better modelling and inclusion of glitches in large-scale studies, such as stress testing the search pipelines and increasing the confidence of detection. In this work, we employ a Generative Adversarial Network (GAN) to produce a particular class of glitches ({\it blip}) in the time domain. We share the trained network through a user-friendly open-source software package called \texttt{gengli} and provide practical examples of its usage.

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Cited by 1 Pith paper

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  1. Null Stream Based Third-generation-ready Glitch Mitigation for Gravitational Wave Measurements

    gr-qc 2024-11 conditional novelty 6.0 of 10

    Using the null stream of a triangular Einstein Telescope, overlapping glitches can be reconstructed and subtracted without signal contamination, preserving parameter estimation accuracy where a two-L-shaped design sho...

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