Discovering features in gravitational-wave data through detector characterization, citizen science and machine learning. (2nd September 2021)

• Record Type: Journal Article
• Authors: Soni, S; Berry, C P L; Coughlin, S B; Harandi, M; Jackson, C B; Crowston, K; Østerlund, C; Patane, O; Katsaggelos, A K; Trouille, L; Baranowski, V-G; Domainko, W F; Kaminski, K; Rodriguez, M A Lobato; Marciniak, U; Nauta, P; Niklasch, G; Rote, R R; Téglás, B; Unsworth, C; Zhang, C
• Is Part Of: Classical and quantum gravity. Volume 38:Number 19(2021)
• Publication Date: 2021-09-02
• Subjects: LIGO -- transient noise -- machine learning -- noise classification -- neural network; Quantum gravity -- Periodicals; Gravitation -- Periodicals; Relativity (Physics) -- Periodicals; Space and time -- Periodicals; Periodicals; 521.1
• DOI: 10.1088/1361-6382/ac1ccb
• Languages: English
• ISSNs: 0264-9381

Abstract

Abstract: The observation of gravitational waves is hindered by the presence of transient noise (glitches). We study data from the third observing run of the Advanced LIGO detectors, and identify new glitch classes: fast scattering/crown and low-frequency blips . Using training sets assembled by monitoring of the state of the detector, and by citizen-science volunteers, we update the Gravity Spy machine-learning algorithm for glitch classification. We find that fast scattering/crown, linked to ground motion at the detector sites, is especially prevalent, and identify two subclasses linked to different types of ground motion. Reclassification of data based on the updated model finds that ∼27% of all transient noise at LIGO Livingston belongs to the fast scattering class, while ∼8% belongs to the low-frequency blip class, making them the most frequent and fourth most frequent sources of transient noise at that site. Our results demonstrate both how glitch classification can reveal potential improvements to gravitational-wave detectors, and how, given an appropriate framework, citizen-science volunteers may make discoveries in large data sets.