The F-statistic is an established method to search for continuous gravitational waves from spinning neutron stars. Prix et al. (2011) introduced a variant for transient quasi-monochromatic signals. Possible astrophysical scenarios for such transients include glitching pulsars, newborn neutron stars and accreting systems. Here we present a new implementation of the transient F-statistic, using pyCUDA to leverage the power of modern graphics processing units (GPUs). The obtained speedup allows efficient searches over much wider parameter spaces, especially when using more realistic transient signal models including time-varying (e.g. exponentially decaying) amplitudes. Hence, it can enable comprehensive coverage of glitches in known nearby pu...
Rapidly spinning neutron stars are promising sources of continuous gravitational waves. Detecting su...
The existence of gravitational waves was predicted by Albert Einstein. Black hole and neutron star b...
Gravitational waves in the sensitivity band of ground-based detectors can be emitted by a number of ...
The F-statistic is an established method to search for continuous gravitational waves from spinning ...
We introduce a search method for a new class of gravitational-wave signals, namely long-duration O(h...
Rapidly rotating, slightly nonaxisymmetric neutron stars emit nearly periodic gravitational waves (G...
A search for long transient gravitational waves associated with neutron stars is presented. The esti...
We describe a method to detect gravitational waves lasting $O(hours-days)$ emitted by young, isolate...
We describe a method to detect gravitational waves lasting O(hours-days) emitted by young, isolated ...
We present a new approach to searching for Continuous gravitational Waves (CWs) emitted by isolated ...
We present a new approach to searching for Continuous gravitational Waves (CWs) emitted by isolated ...
Rapidly spinning neutron stars are promising sources of continuous gravitational waves. Detecting su...
The existence of gravitational waves was predicted by Albert Einstein. Black hole and neutron star b...
Gravitational waves in the sensitivity band of ground-based detectors can be emitted by a number of ...
The F-statistic is an established method to search for continuous gravitational waves from spinning ...
We introduce a search method for a new class of gravitational-wave signals, namely long-duration O(h...
Rapidly rotating, slightly nonaxisymmetric neutron stars emit nearly periodic gravitational waves (G...
A search for long transient gravitational waves associated with neutron stars is presented. The esti...
We describe a method to detect gravitational waves lasting $O(hours-days)$ emitted by young, isolate...
We describe a method to detect gravitational waves lasting O(hours-days) emitted by young, isolated ...
We present a new approach to searching for Continuous gravitational Waves (CWs) emitted by isolated ...
We present a new approach to searching for Continuous gravitational Waves (CWs) emitted by isolated ...
Rapidly spinning neutron stars are promising sources of continuous gravitational waves. Detecting su...
The existence of gravitational waves was predicted by Albert Einstein. Black hole and neutron star b...
Gravitational waves in the sensitivity band of ground-based detectors can be emitted by a number of ...