Continuous gravitational-wave (CW) signals are long-lasting quasi-monochromatic
gravitational-wave signals expected to be emitted by rapidly rotating non-axisymmetric …

Continuous gravitational-wave (CW) signals are long-lasting quasi-monochromatic
gravitational-wave signals expected to be emitted by rapidly rotating non-axisymmetric …

Non-axisymmetries in rotating neutron stars emit quasi-monochromatic gravitational waves.
These long-duration'continuous wave'signals are among the main search targets of ground …

We present a new veto procedure to distinguish between continuous gravitational wave
(CW) signals and the detector artifacts that can mimic their behavior. The veto procedure …

We compute the stochastic gravitational wave (GW) background generated by black hole–
black hole (BH–BH) hyperbolic encounters with eccentricities close to one and compare …

Merger rates of binary black holes, binary neutron stars, and neutron-star–black-hole
binaries in the local Universe (ie, redshift z= 0), inferred from the Laser Interferometer …

In order to separate astrophysical gravitational-wave signals from instrumental noise, which
often contains transient non-Gaussian artifacts, astronomers have traditionally relied on …

Continuous gravitational waves are long-lasting forms of gravitational radiation produced by
persistent quadrupolar variations of matter. Standard expected sources for ground-based …

We show that for detections of gravitational-wave transients, constraints can be given on
physical parameters of the source without using any specific astrophysical models. Relying …

The vulnerability to single-detector instrumental artifacts in standard detection methods for
long-duration quasimonochromatic gravitational waves from nonaxisymmetric rotating …