Application of the independent component analysis to the iKAGRA data
arXiv:1908.03013 · doi:10.1093/ptep/ptaa056
Abstract
We apply the independent component analysis (ICA) to the real data from a gravitational wave detector for the first time. Specifically we use the iKAGRA data taken in April 2016, and calculate the correlations between the gravitational wave strain channel and 35 physical environmental channels. Using a couple of seismic channels which are found to be strongly correlated with the strain, we perform ICA. Injecting a sinusoidal continuous signal in the strain channel, we find that ICA recovers correct parameters with enhanced signal-to-noise ratio, which demonstrates usefulness of this method. Among the two implementations of ICA used here, we find the correlation method yields the optimal result for the case environmental noises act on the strain channel linearly.
arXiv comment27 pages, 12 figures : published in PTEP with added discussion about the relation between ICA and Wiener filtering
References in corpus (28)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Interferometer design of the KAGRA gravitational wave detector
- Detection, Measurement and Gravitational Radiation
- A guide to LIGO-Virgo detector noise and extraction of transient gravitational-wave signals
- Gravity Spy: Integrating Advanced LIGO Detector Characterization, Machine Learning, and Citizen Science
- Fast Automated Analysis of Strong Gravitational Lenses with Convolutional Neural Networks
- The Spitzer Survey of Stellar Structure in Galaxies (SG): Precise Stellar Mass Distributions from Automated Dust Correction at 3.6 microns
- Component separation methods for the Planck mission
- Glitch Classification and Clustering for LIGO with Deep Transfer Learning
- Deep Transfer Learning: A new deep learning glitch classification method for advanced LIGO
- Blind foreground subtraction for intensity mapping experiments
- Mitigation of the instrumental noise transient in gravitational-wave data surrounding GW170817
- Improving astrophysical parameter estimation via offline noise subtraction for Advanced LIGO
- Image-based deep learning for classification of noise transients in gravitational wave detectors
- Repeatability and Accuracy of Exoplanet Eclipse Depths Measured with Post-Cryogenic Spitzer
- Construction of KAGRA: an Underground Gravitational Wave Observatory
- Active noise cancellation in a suspended interferometer
- Parameter Estimation and Model Selection of Gravitational Wave Signals Contaminated by Transient Detector Noise Glitches
- First cryogenic test operation of underground km-scale gravitational-wave observatory KAGRA
- Revisiting Spitzer transit observations with Independent Component Analysis: new results for the GJ436 system
- Regression of Environmental Noise in LIGO Data
- Classifying the unknown: discovering novel gravitational-wave detector glitches using similarity learning
- Increasing LIGO sensitivity by feedforward subtraction of auxiliary length control noise
- Global Feed-Forward Vibration Isolation in a km scale Interferometer
- Probing gravitational wave polarizations with Advanced LIGO, Advanced Virgo and KAGRA
- Repeatability of Spitzer/IRAC exoplanetary eclipses with Independent Component Analysis
- Toward the detection of gravitational waves under non-Gaussian noises II. Independent Component Analysis
- CO Component Estimation Based on the Independent Component Analysis
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- Performance of the KAGRA detector during the first joint observation with GEO 600 (O3GK)
- Stability of the protoneutron stars toward black hole formation
- Method for environmental noise estimation via injection tests for ground-based gravitational wave detectors
- Blind source separation in 3rd generation gravitational-wave detectors
- Nonlinear Independent Component Analysis Scheme and its application to gravitational wave data analysis
- Evaluation of microseismic motion at the KAGRA site based on ocean wave data