Improving the Sensitivity of Advanced LIGO Using Noise Subtraction
arXiv:1809.05348 · doi:10.1088/1361-6382/ab01c5
Abstract
This paper presents an adaptable, parallelizable method for subtracting linearly coupled noise from Advanced LIGO data. We explain the features developed to ensure that the process is robust enough to handle the variability present in Advanced LIGO data. In this work, we target subtraction of noise due to beam jitter, detector calibration lines, and mains power lines. We demonstrate noise subtraction over the entirety of the second observing run, resulting in increases in sensitivity comparable to those reported in previous targeted efforts. Over the course of the second observing run, we see a 30% increase in Advanced LIGO sensitivity to gravitational waves from a broad range of compact binary systems. We expect the use of this method to result in a higher rate of detected gravitational-wave signals in Advanced LIGO data.
arXiv comment15 pages, 6 figures
References in corpus (30)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
- GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
- Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?
- Characterization of the LIGO detectors during their sixth science run
- GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence
- Robust parameter estimation for compact binaries with ground-based gravitational-wave observations using the LALInference software library
- The Black Hole Mass Distribution in the Galaxy
- The PyCBC search for gravitational waves from compact binary coalescence
- The Mass Distribution of Stellar-Mass Black Holes
- BayesWave: Bayesian Inference for Gravitational Wave Bursts and Instrument Glitches
- Coherent method for detection of gravitational wave bursts
- The astrophysical gravitational wave stochastic background
- Identification and mitigation of narrow spectral artifacts that degrade searches for persistent gravitational waves in the first two observing runs of Advanced LIGO
- An information-theoretic approach to the gravitational-wave burst detection problem
- Calibration Uncertainty for Advanced LIGO's First and Second Observing Runs
- Recent searches for continuous gravitational waves
- Reconstructing the calibrated strain signal in the Advanced LIGO detectors
- The Advanced LIGO Photon Calibrators
- A hierarchical method for vetoing noise transients in gravitational-wave detectors
- Improving the Data Quality of Advanced LIGO Based on Early Engineering Run Results
- Overview of Advanced LIGO Adaptive Optics
- Validating gravitational-wave detections: The Advanced LIGO hardware injection system
- Active noise cancellation in a suspended interferometer
- Characterising Transient Noise in the LIGO Detectors
- Neutron stars versus black holes: probing the mass gap with LIGO/Virgo
- Regression of Environmental Noise in LIGO Data
- Global Feed-Forward Vibration Isolation in a km scale Interferometer
- Increasing LIGO sensitivity by feedforward subtraction of auxiliary length control noise
- Identifying correlations between LIGO's astronomical range and auxiliary sensors using lasso regression
Cited by in corpus (80)
- GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
- GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
- GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
- GW190425: Observation of a Compact Binary Coalescence with Total Mass
- Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1
- Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog
- GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses
- Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo
- A guide to LIGO-Virgo detector noise and extraction of transient gravitational-wave signals
- Open data from the third observing run of LIGO, Virgo, KAGRA and GEO
- Search for the isotropic stochastic background using data from Advanced LIGO's second observing run
- 4-OGC: Catalog of gravitational waves from compact-binary mergers
- LIGO Detector Characterization in the Second and Third Observing Runs
- 3-OGC: Catalog of gravitational waves from compact-binary mergers
- Search for sub-solar mass ultracompact binaries in Advanced LIGO's second observing run
- Enhancing Gravitational-Wave Science with Machine Learning
- Search for gravitational waves from a long-lived remnant of the binary neutron star merger GW170817
- Tests of General Relativity with GWTC-3
- Machine-learning non-stationary noise out of gravitational wave detectors
- Searches for Continuous-Wave Gravitational Radiation
- Searches for Gravitational Waves from Known Pulsars at Two Harmonics in 2015-2017 LIGO Data
- On the properties of the massive binary black hole merger GW170729
- Search for intermediate mass black hole binaries in the third observing run of Advanced LIGO and Advanced Virgo
- The curious case of GW200129: interplay between spin-precession inference and data-quality issues
- Noise Reduction in Gravitational-wave Data via Deep Learning
- Narrowband searches for continuous and long-duration transient gravitational waves from known pulsars in the LIGO-Virgo third observing run
- Searches for Gravitational Waves from Known Pulsars at Two Harmonics in the Second and Third LIGO-Virgo Observing Runs
- Subtracting glitches from gravitational-wave detector data during the third observing run
- Environmental Noise in Advanced LIGO Detectors
- Directional limits on persistent gravitational waves using data from Advanced LIGO's first two observing runs
- Search methods for continuous gravitational-wave signals from unknown sources in the advanced-detector era
- Modeling compact binary signals and instrumental glitches in gravitational wave data
- Possible Causes of False General Relativity Violations in Gravitational Wave Observations
- Constraining scalar-tensor theories by neutron star-balck hole gravitational wave events
- Einstein@Home all-sky search for continuous gravitational waves in LIGO O2 public data
- Quantifying the Effect of Power Spectral Density Uncertainty on Gravitational-Wave Parameter Estimation for Compact Binary Sources
- Deep Einstein@Home all-sky search for continuous gravitational waves in LIGO O3 public data
- Accurate modeling and mitigation of overlapping signals and glitches in gravitational-wave data
- Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA
- First search for long-duration transient gravitational waves after glitches in the Vela and Crab pulsars
- All-sky search for long-duration gravitational-wave transients in the second Advanced LIGO observing run
- Revisiting the evidence for precession in GW200129 with machine learning noise mitigation
- Rapid and Robust Parameter Inference for Binary Mergers
- Eccentric or circular? A reanalysis of binary black hole gravitational wave events for orbital eccentricity signatures
- End benches scattered light modeling and subtraction in Advanced Virgo
- Search for binary black hole mergers in the third observing run of Advanced LIGO-Virgo using coherent WaveBurst enhanced with machine learning
- Gaussian Processes for Glitch-robust Gravitational-wave Astronomy
- Efficient parameter inference for gravitational wave signals in the presence of transient noises using temporal and time-spectral fusion normalizing flow
- Convolutional Neural Networks for the classification of glitches in gravitational-wave data streams
- Assessing and Mitigating the Impact of Glitches on Gravitational-Wave Parameter Estimation: a Model Agnostic Approach
- Analyzing black-hole ringdowns II: data conditioning
- Results from an Einstein@Home search for continuous gravitational waves from G347.3 at low frequencies in LIGO O2 data
- Adding equatorial-asymmetric effects for spin-precessing binaries into the SEOBNRv5PHM waveform model
- Enabling multi-messenger astronomy with continuous gravitational waves: early warning and sky localization of binary neutron stars in Einstein Telescope
- Coherence-based approaches for estimating the composition of the seismic wavefield
- Bayesian modelling of scattered light in the LIGO interferometers
- Incorporating information from LIGO data quality streams into the PyCBC search for gravitational waves
- Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run
- Robust inference of gravitational wave source parameters in the presence of noise transients using normalizing flows
- A Sensitive Test of Non-Gaussianity in Gravitational-wave Detector Data
- Gravitational-Wave Parameter Estimation in non-Gaussian noise using Score-Based Likelihood Characterization
- Likelihood for a Network of Gravitational-Wave Detectors with Correlated Noise
- cDVGAN: One Flexible Model for Multi-class Gravitational Wave Signal and Glitch Generation
- Calibration of Advanced Virgo and reconstruction of detector strain h(t) during the Observing Run O3
- DeepExtractor: Time-domain reconstruction of signals and glitches in gravitational wave data with deep learning
- Null Stream Based Third-generation-ready Glitch Mitigation for Gravitational Wave Measurements
- Detecting and Diagnosing Terrestrial Gravitational-Wave Mimics Through Feature Learning
- All-sky search for long-duration gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run
- Search for continuous gravitational waves from unknown neutron stars in binary systems with long orbital periods in O3 data
- Joint inference for gravitational wave signals and glitches using a data-informed glitch model
- Glitches far from transient gravitational-wave events do not bias inference
- Einstein@Home all-sky "bucket" search for continuous gravitational waves in LIGO O3 public data
- Impact of noise transients on gravitational-wave burst detection efficiency of the BayesWave pipeline with multi-detector networks
- Application of Non-Linear Noise Regression in the Virgo Detector
- Bayesian Framework to Follow-up Continuous Gravitational Wave Candidates from Deep Surveys
- High-frequency continuous gravitational waves searched in LIGO O3 public data with Einstein@Home
- Narrowband searches for continuous gravitational waves from known pulsars in the first two parts of the fourth LIGO--Virgo--KAGRA observing run
- Identification of Noise-Associated Glitches in KAGRA O3GK with Hveto
- Nonlinear Independent Component Analysis Scheme and its application to gravitational wave data analysis
- Extending Ground-Based Gravitational-Wave Sensitivity to 5 Hz