We describe a new technique for removing troublesome interference from external coherent signals present in the gravitational wave spectrum. The method works when the interference is present in many harmonics, as long as they remain coherent with one another. The method can remove interference even when the frequency changes. We apply the method to the data produced by the Glasgow laser interferometer in 1996 and the entire series of wide lines corresponding to the electricity supply frequency and its harmonics are removed, leaving the spectrum clean enough to detect possible signals previously masked by them. We also study the effects of the line removal on the statistics of the noise in the time domain. We find that this technique seems t...
We consider a recent scheme of gravitational wave detection using atomic interferometers a...
One of the major obstacles to the detection and study of gravitational waves using ground-based lase...
The possibility of measuring the second order correlation function of the gravitational waves detect...
We describe a new technique for removing troublesome interference from external coherent signals pre...
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 non-stationary and non-harmonic interferen...
We develop a procedure to remove interference from gravitational wave spectrum. The method is applie...
We describe a procedure to identify and remove a class of nonstationary and nonharmonic interference...
I present a new method to remove detector noise from gravitationalwave (GW) interferometer data in t...
Many experiments, and in particular gravitational wave detectors, produce continuous streams of data...
The operation of 106 km scale laser interferometers in space will permit the detection of gravitatio...
We describe a tool we improved to detect excess noise in the gravitational wave (GW) channel arising...
It is known by the experience gained from the gravitational wave detector prototypes that the interf...
The sensitivity of next-generation gravitational-wave detectors such as Advanced LIGO and LCGT shoul...
High power in narrow frequency bands, spectral lines, are a feature of an interferometric gravitatio...
We consider a recent scheme of gravitational wave detection using atomic interferometers a...
One of the major obstacles to the detection and study of gravitational waves using ground-based lase...
The possibility of measuring the second order correlation function of the gravitational waves detect...
We describe a new technique for removing troublesome interference from external coherent signals pre...
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 non-stationary and non-harmonic interferen...
We develop a procedure to remove interference from gravitational wave spectrum. The method is applie...
We describe a procedure to identify and remove a class of nonstationary and nonharmonic interference...
I present a new method to remove detector noise from gravitationalwave (GW) interferometer data in t...
Many experiments, and in particular gravitational wave detectors, produce continuous streams of data...
The operation of 106 km scale laser interferometers in space will permit the detection of gravitatio...
We describe a tool we improved to detect excess noise in the gravitational wave (GW) channel arising...
It is known by the experience gained from the gravitational wave detector prototypes that the interf...
The sensitivity of next-generation gravitational-wave detectors such as Advanced LIGO and LCGT shoul...
High power in narrow frequency bands, spectral lines, are a feature of an interferometric gravitatio...
We consider a recent scheme of gravitational wave detection using atomic interferometers a...
One of the major obstacles to the detection and study of gravitational waves using ground-based lase...
The possibility of measuring the second order correlation function of the gravitational waves detect...