I present a new method to remove detector noise from gravitationalwave (GW) interferometer data in the framework of unmodeled analyses, with special reference to coherent WaveBurst pipeline. The method introduces a pixel selection rule in the time-frequency representation of multidetector data to exclude noisy time-frequency components: this is performed multiplying each pixel by a weight function ranging from 0 to 1 and based on the coherence of the data among the detectors. Preliminary simulations indicate an improved suppression of noise with better reconstruction of both polarization components of detected GW signals
We describe a procedure to identify and remove a class of interference lines from gravitational wave...
We describe a procedure to identify and remove a class of nonstationary and nonharmonic interference...
International audienceThe detection of Galactic binaries as sources of gravitational waves promises ...
We describe a new technique for removing troublesome interference from external coherent signals pre...
One of the goals of gravitational data wave analysis is the knowledge and accurate estimation of the...
It is known by the experience gained from the gravitational wave detector prototypes that the interf...
International audienceEstimating the parameters of gravitational wave signals detected by ground-bas...
Orbiting compact binaries - such as binary black holes, binary neutron stars and neutron star-black ...
The data collected by the current network of gravitational-wave detectors are largely dominated by i...
Signal extraction out of background noise is a common challenge in high-precision physics experiment...
We propose an adaptive denoising scheme for poorly modeled non-Gaussian features in the gravitationa...
The detection of unmodeled gravitational wave transients (bursts) using a network of interferometric...
It is expected that interferometric gravitational wave detectors such as LIGO \cite{Barish99} will b...
Current gravitational wave searches for compact binaries coalescence are done using a bank of templa...
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 interference lines from gravitational wave...
We describe a procedure to identify and remove a class of nonstationary and nonharmonic interference...
International audienceThe detection of Galactic binaries as sources of gravitational waves promises ...
We describe a new technique for removing troublesome interference from external coherent signals pre...
One of the goals of gravitational data wave analysis is the knowledge and accurate estimation of the...
It is known by the experience gained from the gravitational wave detector prototypes that the interf...
International audienceEstimating the parameters of gravitational wave signals detected by ground-bas...
Orbiting compact binaries - such as binary black holes, binary neutron stars and neutron star-black ...
The data collected by the current network of gravitational-wave detectors are largely dominated by i...
Signal extraction out of background noise is a common challenge in high-precision physics experiment...
We propose an adaptive denoising scheme for poorly modeled non-Gaussian features in the gravitationa...
The detection of unmodeled gravitational wave transients (bursts) using a network of interferometric...
It is expected that interferometric gravitational wave detectors such as LIGO \cite{Barish99} will b...
Current gravitational wave searches for compact binaries coalescence are done using a bank of templa...
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 interference lines from gravitational wave...
We describe a procedure to identify and remove a class of nonstationary and nonharmonic interference...
International audienceThe detection of Galactic binaries as sources of gravitational waves promises ...