Detection of anomalies amongst LIGO's glitch populations with autoencoders
Paloma Laguarta, Robin van der Laag, Melissa Lopez, Tom Dooney, Andrew, L. Miller, Stefano Schmidt, Marco Cavaglia, Sarah Caudill, Kurt Driessens,, J\"oel Karel, Roy Lenders, Chris Van Den Broeck

TL;DR
This paper introduces an unsupervised autoencoder-based method utilizing fractal dimension encoding of auxiliary channels to identify and analyze unknown glitch anomalies in LIGO gravitational-wave data, improving glitch detection capabilities.
Contribution
The work presents a novel unsupervised framework combining fractal dimension encoding and autoencoders to detect unknown glitches using auxiliary channel data in LIGO.
Findings
Discovered anomalies in 6.6% of data
Uncovered unknown glitch morphologies
Enhanced glitch identification framework
Abstract
Gravitational-wave (GW) interferometers are able to detect a change in distance of 1/10,000th the size of a proton. Such sensitivity leads to large appearance rates of non-Gaussian transient noise bursts in the main detector strain, also known as glitches. These glitches come in a wide range of frequency-amplitude-time morphologies and are caused by environmental or instrumental processes, hindering searches for all sources of gravitational waves. Current approaches for their identification use supervised models to learn their morphology in the main strain, but do not consider relevant information provided by auxiliary channels that monitor the state of the interferometers nor provide a flexible framework for novel glitch morphologies. In this work, we present an unsupervised algorithm to find anomalous glitches. We encode a subset of auxiliary channels from LIGO Livingston in…
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Taxonomy
TopicsTime Series Analysis and Forecasting · Complex Systems and Time Series Analysis · Computational Physics and Python Applications
