Classification methods for noise transients in advanced gravitational-wave detectors II: performance tests on Advanced LIGO data
Jade Powell, Alejandro Torres-Forn\'e, Ryan Lynch, Daniele Trifir\`o,, Elena Cuoco, Marco Cavagli\`a, Ik Siong Heng, Jos\'e A. Font

TL;DR
This paper evaluates three noise transient classification methods for advanced LIGO data, demonstrating their high accuracy and benefits of combined classifiers to improve gravitational-wave detector data analysis.
Contribution
First performance tests of three transient noise classification algorithms on real LIGO data, with improvements for real-time application and non-stationary noise conditions.
Findings
All methods classify transients with high accuracy.
Using multiple classifiers improves performance.
Algorithms are ready for second observation run.
Abstract
The data taken by the advanced LIGO and Virgo gravitational-wave detectors contains short duration noise transients that limit the significance of astrophysical detections and reduce the duty cycle of the instruments. As the advanced detectors are reaching sensitivity levels that allow for multiple detections of astrophysical gravitational-wave sources it is crucial to achieve a fast and accurate characterization of non-astrophysical transient noise shortly after it occurs in the detectors. Previously we presented three methods for the classification of transient noise sources. They are Principal Component Analysis for Transients (PCAT), Principal Component LALInference Burst (PC-LIB) and Wavelet Detection Filter with Machine Learning (WDF-ML). In this study we carry out the first performance tests of these algorithms on gravitational-wave data from the Advanced LIGO detectors. We use…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
