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 interpretation of pulsar rotational glitches, the sudden increase in spin frequency of
neutron stars, is a half-century-old challenge. The common view is that glitches are driven by …

The Advanced LIGO [1] and Advanced Virgo [2] detectors have made numerous detections
of gravitational waves (GWs), to date consisting of short-duration (transient) GWs emitted …

Abstract Machine learning has emerged as a popular and powerful approach for solving
problems in astrophysics. We review applications of machine learning techniques for the …

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 …

Continuous gravitational waves (CWs) are quasi-monochromatic signals expected to be
ever-present in the data of gravitational-wave (GW) detectors such as Advanced LIGO (Aasi …

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

Direct detection of gravitational waves has become a powerful new tool of multi-messenger
astrophysics. Apart from short-duration (transient) events, such as the inspirals and mergers …

Gravitational waves can probe the existence of planetary-mass primordial black holes.
Considering a mass range of [1 0− 7− 1 0− 2] M⊙, inspiraling primordial black holes could …

The young (1–5 kyr) energetic pulsar PSR J0537− 6910 (Wang & Gotthelf 1998; Chen et al.
2006) resides in the Large Magellanic Cloud at a distance of 49.6 kpc (Pietrzyński et al …