Magnetars are young and highly magnetized neutron stars that display a wide array of X-ray
activity including short bursts, large outbursts, giant flares, and quasi-periodic oscillations …

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 …

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 …

Radio pulsars provide us with some of the most stable clocks in the universe. Nevertheless
several pulsars exhibit sudden spin-up events, known as glitches. More than forty years after …

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 …

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 …

∼ 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 …

We present a phase-coherent timing solution for PSR J1640–4631, a young 206 ms pulsar
using X-ray timing observations taken with NuSTAR. Over this timing campaign, we have …

Magnetars are neutron stars with X-ray and soft γ-ray outbursts thought to be powered by
intense internal magnetic fields. Like conventional neutron stars in the form of radio pulsars …