The discovery of pulsars opened a new research field that allows studying a wide range of
physics under extreme conditions. More than 3,000 pulsars are currently known, including …

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 …

There have been several previous searches for persistent (or continuous) quasi-
monochromatic gravitational waves emitted by a selection of known pulsars using data from …

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 …

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 …

The 2016 Vela glitch observed by the Mount Pleasant radio telescope provides the first
opportunity to study pulse-to-pulse dynamics of a pulsar glitch, opening up new possibilities …

While pulsars possess exceptional rotational stability, large-scale timing studies have
revealed at least two distinct types of irregularities in their rotation: red timing noise and …

Neutron stars are compact and dense celestial objects that offer the unique opportunity to
explore matter and its interactions under conditions that cannot be reproduced elsewhere in …

Isolated spinning neutron stars, asymmetric with respect to their rotation axis, are expected
to be sources of continuous gravitational waves. The most sensitive searches for these …