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 …

Pulsar timing arrays (PTAs) are galactic-scale gravitational wave (GW) detectors. Each
individual arm, composed of a millisecond pulsar, a radio telescope, and a kiloparsecs-long …

∼ 6% of all known pulsars have been observed to exhibit sudden spin-up events, known as
glitches. For more than fifty years, these phenomena have played an important role in …

This paper presents the results of a search for generic short-duration gravitational-wave
transients in data from the third observing run of Advanced LIGO and Advanced Virgo …

Over the last 40 years, an astonishing range of astrophysics has become accessible through
pulsar astronomy. The body of literature on this rapidly growing research area is vast and …

We report on a timing programme of 74 young pulsars that have been observed by the
Parkes 64-m radio telescope over the past decade. Using modern Bayesian timing …

Pulsar glitches are rapid spin-up events that occur in the rotation of neutron stars, providing
a valuable probe into the physics of the interiors of these objects. Long-term monitoring of a …

Two recent discoveries, namely PSR J0901− 4046 and GLEAM-X J162759. 5− 523504.3
(hereafter GLEAM-X J1627), have corroborated an extant population of radio-loud periodic …

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 …

Among the various oscillation modes of neutron stars, f-and g-modes are the most likely to
be ultimately observed in binary neutron star mergers due to their relatively large coupling …