April 25, 2024, 7:43 p.m. | Yi Li, Yunan Wu, Aggelos K. Katsaggelos

cs.LG updates on arXiv.org arxiv.org

arXiv:2404.15552v1 Announce Type: cross
Abstract: The advancement of The Laser Interferometer Gravitational-Wave Observatory (LIGO) has significantly enhanced the feasibility and reliability of gravitational wave detection. However, LIGO's high sensitivity makes it susceptible to transient noises known as glitches, which necessitate effective differentiation from real gravitational wave signals. Traditional approaches predominantly employ fully supervised or semi-supervised algorithms for the task of glitch classification and clustering. In the future task of identifying and classifying glitches across main and auxiliary channels, it is …

arxiv astro-ph.im autoencoder clustering cs.cv cs.lg dimensionality gr-qc spectrogram temporal type unsupervised

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