One of the types of signals for which the LIGO interferometric gravitational wave detectors will search is a stochastic background of gravitational radiation. We review the technique of searching for a background using the optimally-filtered cross-correlation statistic, and describe the state of plans to perform such cross-correlations between the two LIGO interferometers as well as between LIGO and other gravitational-wave detectors, in particular the preparation of software to perform such data analysis
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...
We consider the question of cross-correlation measurements using Virgo and the LSC Interferometers (...
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...
One of the types of signals for which the LIGO interferometric gravitational wave detectors will sea...
We describe the role of correlation measurements between the LIGO interferometer in Livingston, LA, ...
We analyze the signal processing required for the optimal detection of a stochastic background of gr...
I describe analysis of correlations in the outputs of the three LIGO interferometers from LIGO's fir...
We describe the utility of simulated-signal injection studies on earth-based gravitational-wave (GW)...
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...
We consider the question of cross-correlation measurements using Virgo and the LSC Interferometers (...
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...
One of the types of signals for which the LIGO interferometric gravitational wave detectors will sea...
We describe the role of correlation measurements between the LIGO interferometer in Livingston, LA, ...
We analyze the signal processing required for the optimal detection of a stochastic background of gr...
I describe analysis of correlations in the outputs of the three LIGO interferometers from LIGO's fir...
We describe the utility of simulated-signal injection studies on earth-based gravitational-wave (GW)...
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...
We consider the question of cross-correlation measurements using Virgo and the LSC Interferometers (...
The stochastic gravitational-wave background is a superposition of sources that are either too weak ...