Detecting and Diagnosing Terrestrial Gravitational-Wave Mimics Through Feature Learning
arXiv:2203.05086 · doi:10.1103/PhysRevD.107.062006
Abstract
As engineered systems grow in complexity, there is an increasing need for automatic methods that can detect, diagnose, and even correct transient anomalies that inevitably arise and can be difficult or impossible to diagnose and fix manually. Among the most sensitive and complex systems of our civilization are the detectors that search for incredibly small variations in distance caused by gravitational waves -- phenomena originally predicted by Albert Einstein to emerge and propagate through the universe as the result of collisions between black holes and other massive objects in deep space. The extreme complexity and precision of such detectors causes them to be subject to transient noise issues that can significantly limit their sensitivity and effectiveness. In this work, we present a demonstration of a method that can detect and characterize emergent transient anomalies of such massively complex systems. We illustrate the performance, precision, and adaptability of the automated solution via one of the prevalent issues limiting gravitational-wave discoveries: noise artifacts of terrestrial origin that contaminate gravitational wave observatories' highly sensitive measurements and can obscure or even mimic the faint astrophysical signals for which they are listening. Specifically, we demonstrate how a highly interpretable convolutional classifier can automatically learn to detect transient anomalies from auxiliary detector data without needing to observe the anomalies themselves. We also illustrate several other useful features of the model, including how it performs automatic variable selection to reduce tens of thousands of auxiliary data channels to only a few relevant ones; how it identifies behavioral signatures predictive of anomalies in those channels; and how it can be used to investigate individual anomalies and the channels associated with them.
References in corpus (46)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- Multi-messenger Observations of a Binary Neutron Star Merger
- GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
- Advanced LIGO
- GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
- Sensitivity and Performance of the Advanced LIGO Detectors in the Third Observing Run
- Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914
- New binary black hole mergers in the second observing run of Advanced LIGO and Advanced Virgo
- Gravity Spy: Integrating Advanced LIGO Detector Characterization, Machine Learning, and Citizen Science
- 2-OGC: Open Gravitational-wave Catalog of binary mergers from analysis of public Advanced LIGO and Virgo data
- Multiresolution techniques for the detection of gravitational-wave bursts
- LIGO Detector Characterization in the Second and Third Observing Runs
- Seismic isolation of Advanced LIGO: Review of strategy, instrumentation and performance
- A Highly Spinning and Aligned Binary Black Hole Merger in the Advanced LIGO First Observing Run
- 1-OGC: The first open gravitational-wave catalog of binary mergers from analysis of public Advanced LIGO data
- 3-OGC: Catalog of gravitational waves from compact-binary mergers
- Enhancing Gravitational-Wave Science with Machine Learning
- Machine-learning non-stationary noise out of gravitational wave detectors
- GEO 600 and the GEO-HF upgrade program: successes and challenges
- Improving the Sensitivity of Advanced LIGO Using Noise Subtraction
- Application of machine learning algorithms to the study of noise artifacts in gravitational-wave data
- Reducing Scattered Light in LIGO's Third Observing Run
- The LSC Glitch Group : Monitoring Noise Transients during the fifth LIGO Science Run
- Detecting Gravitational Waves With Disparate Detector Responses: Two New Binary Black Hole Mergers
- Image-based deep learning for classification of noise transients in gravitational wave detectors
- The characterization of Virgo data and its impact on gravitational-wave searches
- A hierarchical method for vetoing noise transients in gravitational-wave detectors
- Sensors and Actuators for the Advanced LIGO Mirror Suspensions
- Improving the Data Quality of Advanced LIGO Based on Early Engineering Run Results
- Transient Classification in LIGO data using Difference Boosting Neural Network
- Environmental Noise in Advanced LIGO Detectors
- Finding the origin of noise transients in LIGO data with machine learning
- Efficient Gravitational-wave Glitch Identification from Environmental Data Through Machine Learning
- Utilizing aLIGO Glitch Classifications to Validate Gravitational-Wave Candidates
- Large-angle scattered light measurements for quantum-noise filter cavity design studies
- Transient glitch mitigation in Advanced LIGO data with
- Optimizing Vetoes for Gravitational-wave Transient Searches
- Improving the Robustness of the Advanced LIGO Detectors to Earthquakes
- Gwadaptive_scattering: an automated pipeline for scattered light noise characterization
- Search for Advanced LIGO Single Interferometer Compact Binary Coalescence Signals in Coincidence with Gamma-Ray Events in Fermi-GBM
- A Coincidence Null Test for Poisson-Distributed Events
- Effects of transients in LIGO suspensions on searches for gravitational waves
- Application of a new transient-noise analysis tool for an unmodeled gravitational-wave search pipeline
- Architectural Optimization and Feature Learning for High-Dimensional Time Series Datasets