Recent advances in ground‐based interferometric gravitational wave detectors have produced a high level of confidence in detection of transient gravitational wave signals generated by coalescing neutron star or black hole binaries. The combination of gravitational wave data and associated electromagnetic radiation observed by telescopes will allow precision testing of general relativity, including measurement of the speed of gravitational waves. We present a new method of detection based on Infinite Impulse response (IIR) filtering with the goal of computing signal to noise ratios in near real time (low‐latency). We then apply a set of IIR filters to the incoming detector data and coherent sum the outputs to produce near optimal signal to n...
Gravitational waves are a consequence of the general theory of relativity. Direct detection of such...
We compute the sensitivity, constrained by instrumental, propagation, and other fundamental noises, ...
The observational era of gravitational-wave astronomy began in the fall of 2015 with the detection o...
With the upgrade of current gravitational wave detectors, the first detection of gravitational wave ...
Electromagnetic (EM) follow-up observations of gravitational wave events will help shed light on the...
Low-latency event triggers to signify the presence of gravitational waves from coalescing binaries w...
Joint electromagnetic and gravitational-wave (GW) observation is a major goal of both the GW astrono...
Typical sources of gravitational wave bursts are supernovae, for which no accurate models exist. Thi...
We study in this paper some filters for the detection of burst-like signals in the data of interfero...
The reliability of the first detection is one of the most interesting challenges for the gravitation...
Filters developed in order to detect short bursts of gravitational waves in interferometric detector...
Using optimal matched filtering, we search 25 hours of data from the LIGO 40-m prototype laser inter...
As two neutron stars merge, they emit gravitational waves that can potentially be detected by earth ...
We show that gravitational-wave signals from compact binary mergers may be better distinguished from...
Searches for known waveforms in gravitational wave detector data are often done using matched filter...
Gravitational waves are a consequence of the general theory of relativity. Direct detection of such...
We compute the sensitivity, constrained by instrumental, propagation, and other fundamental noises, ...
The observational era of gravitational-wave astronomy began in the fall of 2015 with the detection o...
With the upgrade of current gravitational wave detectors, the first detection of gravitational wave ...
Electromagnetic (EM) follow-up observations of gravitational wave events will help shed light on the...
Low-latency event triggers to signify the presence of gravitational waves from coalescing binaries w...
Joint electromagnetic and gravitational-wave (GW) observation is a major goal of both the GW astrono...
Typical sources of gravitational wave bursts are supernovae, for which no accurate models exist. Thi...
We study in this paper some filters for the detection of burst-like signals in the data of interfero...
The reliability of the first detection is one of the most interesting challenges for the gravitation...
Filters developed in order to detect short bursts of gravitational waves in interferometric detector...
Using optimal matched filtering, we search 25 hours of data from the LIGO 40-m prototype laser inter...
As two neutron stars merge, they emit gravitational waves that can potentially be detected by earth ...
We show that gravitational-wave signals from compact binary mergers may be better distinguished from...
Searches for known waveforms in gravitational wave detector data are often done using matched filter...
Gravitational waves are a consequence of the general theory of relativity. Direct detection of such...
We compute the sensitivity, constrained by instrumental, propagation, and other fundamental noises, ...
The observational era of gravitational-wave astronomy began in the fall of 2015 with the detection o...