Automated Evaluation of Environmental Coupling for Advanced LIGO Gravitational Wave Detections
arXiv:2312.00735 · doi:10.1088/1361-6382/ad5139
Abstract
The extreme sensitivity required for direct observation of gravitational waves by the Advanced LIGO detectors means that environmental noise is increasingly likely to contaminate Advanced LIGO gravitational wave signals if left unaddressed. Consequently, environmental monitoring efforts have been undertaken and novel noise mitigation techniques have been developed which have reduced environmental coupling and made it possible to analyze environmental artifacts with potential to affect the 90 gravitational wave events detected from 2015-2020 by the Advanced LIGO detectors. So far, there is no evidence for environmental contamination in gravitational wave detections. However, automated, rapid ways to monitor and assess the degree of environmental coupling between gravitational wave detectors and their surroundings are needed as the rate of detections continues to increase. We introduce a computational tool, PEMcheck, for quantifying the degree of environmental coupling present in gravitational wave signals using data from the extant collection of environmental monitoring sensors at each detector. We find that PEMcheck's automated analysis identifies only a small number of gravitational waves that merit further study by environmental noise experts due to possible contamination, a substantial improvement over the manual vetting that occurred for every gravitational wave candidate in the first two observing runs. With the validation provided herein; PEMcheck will play a critical role in event validation during LIGO's fourth observing run as an integral part of the data quality report produced for each gravitational wave candidate.
26 pages, 9 figures. Copy of accepted manuscript
References in corpus (33)
- 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
- GW190814: Gravitational Waves from the Coalescence of a 23 M Black Hole with a 2.6 M Compact Object
- GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
- GW190521: A Binary Black Hole Merger with a Total Mass of
- Observation of gravitational waves from two neutron star-black hole coalescences
- An improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
- Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo
- Method for detection and reconstruction of gravitational wave transients with networks of advanced detectors
- Sensitivity and Performance of the Advanced LIGO Detectors in the Third Observing Run
- Analysis Framework for the Prompt Discovery of Compact Binary Mergers in Gravitational-wave Data
- Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914
- Open data from the third observing run of LIGO, Virgo, KAGRA and GEO
- Multiresolution techniques for the detection of gravitational-wave bursts
- LIGO Detector Characterization in the Second and Third Observing Runs
- Constraints on cosmic strings using data from the third Advanced LIGO-Virgo observing run
- Constraint Likelihood analysis for a network of gravitational wave detectors
- Low-latency analysis pipeline for compact binary coalescences in the advanced gravitational wave detector era
- PyCBC Live: Rapid Detection of Gravitational Waves from Compact Binary Mergers
- Counting And Confusion: Bayesian Rate Estimation With Multiple Populations
- General-relativistic precession in a black-hole binary
- Reducing Scattered Light in LIGO's Third Observing Run
- Summed Parallel Infinite Impulse Response (SPIIR) Filters For Low-Latency Gravitational Wave Detection
- Environmental Noise in Advanced LIGO Detectors
- Environmental Influences on the LIGO Gravitational Wave Detectors during the 6th Science Run
- Point absorbers in Advanced LIGO
- Correlated 1-1000 Hz magnetic field fluctuations from lightning over earth-scale distances and their impact on gravitational wave searches
- Noise in the LIGO Livingston Gravitational Wave Observatory due to Trains
- Effects of lightning strokes on underground gravitational waves observatories