Efficient Gravitational-wave Glitch Identification from Environmental Data Through Machine Learning
Robert E. Colgan, K. Rainer Corley, Yenson Lau, Imre Bartos, and John N. Wright, Zsuzsa Marka, Szabolcs Marka

TL;DR
This paper introduces a machine learning method that analyzes environmental and instrumental data channels to identify glitches in LIGO gravitational wave detectors, reducing false alarms and improving detection confidence.
Contribution
The novel approach leverages all environmental and detector data channels for glitch identification, surpassing previous methods limited to gravitational wave data alone.
Findings
Reduces false alarm rate in gravitational wave detection
Enhances LIGO detector sensitivity and reliability
Successfully monitors all environmental and instrumental channels
Abstract
The LIGO observatories detect gravitational waves through monitoring changes in the detectors' length down to below \, variation---a small fraction of the size of the atoms that make up the detector. To achieve this sensitivity, the detector and its environment need to be closely monitored. Beyond the gravitational wave data stream, LIGO continuously records hundreds of thousands of channels of environmental and instrumental data in order to monitor for possibly minuscule variations that contribute to the detector noise. A particularly challenging issue is the appearance in the gravitational wave signal of brief, loud noise artifacts called ``glitches,'' which are environmental or instrumental in origin but can mimic true gravitational waves and therefore hinder sensitivity. Currently they are primarily identified by analysis of the gravitational wave data stream.…
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