We describe a procedure to identify and remove a class of nonstationary and nonharmonic interference lines from gravitational wave interferometer data. These lines appear to be associated with the external electricity main supply, but their amplitudes are non-stationary and they do not appear at harmonics of the fundamental supply frequency. We find an empirical model able to represent coherently all the nonharmonic lines we have found in the power spectrum, in terms of an assumed reference signal of the “primary” supply input signal. If this signal is not available then it can be reconstructed from the same data by making use of the coherent line removal algorithm that we have described elsewhere. All these lines are broadened by frequency...
We propose an adaptive denoising scheme for poorly modeled non-Gaussianfeatures in the gravitational...
Orbiting compact binaries - such as binary black holes, binary neutron stars and neutron star-black ...
We describe a tool we improved to detect excess noise in the gravitational wave (GW) channel arising...
We describe a procedure to identify and remove a class of non-stationary and non-harmonic interferen...
We describe a procedure to identify and remove a class of nonstationary and nonharmonic interference...
We describe a procedure to identify and remove a class of interference lines from gravitational wave...
We describe a new technique for removing troublesome interference from external coherent signals pre...
We develop a procedure to remove interference from gravitational wave spectrum. The method is applie...
It is known by the experience gained from the gravitational wave detector prototypes that the interf...
Many experiments, and in particular gravitational wave detectors, produce continuous streams of data...
Signal extraction out of background noise is a common challenge in high-precision physics experiment...
I present a new method to remove detector noise from gravitationalwave (GW) interferometer data in t...
It is known by the experience gained from the gravitational wave detector prototypes that the interf...
Data taken by the gravitational wave detector GEO 600 (Danzmann K et al 1994 GEO 600—Proposal for a ...
This article analyzes the data for the first three gravitational wave (GW) events detected in both H...
We propose an adaptive denoising scheme for poorly modeled non-Gaussianfeatures in the gravitational...
Orbiting compact binaries - such as binary black holes, binary neutron stars and neutron star-black ...
We describe a tool we improved to detect excess noise in the gravitational wave (GW) channel arising...
We describe a procedure to identify and remove a class of non-stationary and non-harmonic interferen...
We describe a procedure to identify and remove a class of nonstationary and nonharmonic interference...
We describe a procedure to identify and remove a class of interference lines from gravitational wave...
We describe a new technique for removing troublesome interference from external coherent signals pre...
We develop a procedure to remove interference from gravitational wave spectrum. The method is applie...
It is known by the experience gained from the gravitational wave detector prototypes that the interf...
Many experiments, and in particular gravitational wave detectors, produce continuous streams of data...
Signal extraction out of background noise is a common challenge in high-precision physics experiment...
I present a new method to remove detector noise from gravitationalwave (GW) interferometer data in t...
It is known by the experience gained from the gravitational wave detector prototypes that the interf...
Data taken by the gravitational wave detector GEO 600 (Danzmann K et al 1994 GEO 600—Proposal for a ...
This article analyzes the data for the first three gravitational wave (GW) events detected in both H...
We propose an adaptive denoising scheme for poorly modeled non-Gaussianfeatures in the gravitational...
Orbiting compact binaries - such as binary black holes, binary neutron stars and neutron star-black ...
We describe a tool we improved to detect excess noise in the gravitational wave (GW) channel arising...