The discovery of radio pulsars over a half century ago was a seminal moment in astronomy.
It demonstrated the existence of neutron stars, gave a powerful observational tool to study …

We summarize our current knowledge of neutron-star masses and radii. Recent
instrumentation and computational advances have resulted in a rapid increase in the …

The high-frequency radio sky is bursting with synchrotron transients from massive stellar
explosions and accretion events, but the low-frequency radio sky has, so far, been quiet …

Fast radio bursts (FRBs) are brief radio emissions from distant astronomical sources. Some
are known to repeat, but most are single bursts. Nonrepeating FRB observations have had …

Here we present a catalogue of known Fast Radio Burst (FRB) sources in the form of an
online catalogue, FRBCAT. The catalogue includes information about the instrumentation …

Discovery of pulsars is one of the main goals for large radio telescopes. The Five-hundred-
meter Aperture Spherical radio Telescope (FAST), that incorporates an L-band 19-beam …

The highly stable spin of neutron stars can be exploited for a variety of (astro) physical
investigations. In particular, arrays of pulsars with rotational periods of the order of …

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 …

Searches for transient astrophysical sources often reveal unexpected classes of objects that
are useful physical laboratories. In a recent survey for pulsars and fast transients, we have …

Improving survey specifications are causing an exponential rise in pulsar candidate
numbers and data volumes. We study the candidate filters used to mitigate these problems …