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

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 …

Gravitational waves (GWs) can offer a novel window into the structure and dynamics of
neutron stars. Here we present the first search for long-duration quasimonochromatic GW …

ABSTRACT A systematic, semi-automated search for pulsar glitches in the first UTMOST
public data release is presented. The search is carried out using a hidden Markov model …

Pulsar timing experiments typically generate a phase-connected timing solution from a
sequence of times of arrival (TOAs) by absolute pulse numbering, ie, by fitting an integer …

The interglitch timing of the Vela pulsar is characterized by a constant second derivative of
the rotation rate. This takes over after the post-glitch exponential relaxation and is completed …

The abrupt change in the pulse period of a pulsar is called a pulsar glitch. In this paper, we
present 11 pulsar glitches detected using the Ooty Radio Telescope (ORT) and the …

Isolated neutron stars that are asymmetric with respect to their spin axis are possible
sources of detectable continuous gravitational waves. This paper presents a fully-coherent …

We have observed the Vela pulsar for 1 year using a phased array feed receiver on the 12-
m antenna of the Parkes Test-Bed Facility. These observations have allowed us to …