Now that detection of gravitational-wave signals from the coalescence of extra-galactic
compact binary star mergers has become nearly routine, it is intriguing to consider other …

The birth of gravitational wave astronomy was triggered by the first detection of a signal
produced by the merger of two compact objects (also known as a compact binary …

Abstract The third Gravitational-Wave Transient Catalog (GWTC-3) describes signals
detected with Advanced LIGO and Advanced Virgo up to the end of their third observing run …

This paper describes the first all-sky search for long-duration, quasimonochromatic
gravitational-wave signals emitted by ultralight scalar boson clouds around spinning black …

We present a directed search for continuous gravitational wave (CW) signals emitted by
spinning neutron stars located in the inner parsecs of the Galactic Center (GC). Compelling …

Results are presented of searches for continuous gravitational waves from 20 accreting
millisecond x-ray pulsars with accurately measured spin frequencies and orbital parameters …

We study the prospects for the detection of continuous gravitational signals from normal
Galactic neutron stars, ie, nonrecycled stars. We use a synthetic population generated by …

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

The Virgo detector, based at the EGO (European Gravitational Observatory) and located in
Cascina (Pisa), played a significant role in the development of the gravitational-wave …

Seven years after the first direct detection of gravitational waves, from the collision of two
black holes, the field of gravitational wave astronomy is firmly established. A first detection of …