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 …

Young and rotation-powered neutron stars (NSs) are commonly observed as rapidly-
spinning pulsars. They dissipate their rotational energy by emitting pulsar wind with …

Detections from the repeating fast radio burst FRB 121102 are clustered in time, noticeable
even in the earliest repeat bursts. Recently, it was argued that the source activity is periodic …

Low frequency radio waves, while challenging to observe, are a rich source of information
about pulsars. The LOw Frequency ARray (LOFAR) is a new radio interferometer operating …

We investigate rotational spin noise (referred to as timing noise) in non-accreting pulsars:
millisecond pulsars, canonical pulsars, and magnetars. Particular attention is placed on …

We describe observations of Rotating Radio Transients (RRATs) that were discovered in a
re-analysis of the Parkes Multibeam Pulsar Survey (PMPS). The sources have now been …

Rotation-powered radio pulsars are generally observed to pulse regularly in the radio band,
but this is not the case for so-called rotating radio transients (RRATs) which emit only …

In a search for radio pulsations from the magnetar 1E 1841–045, we have discovered the
unrelated pulsar J1841–0500, with rotation period P= 0.9 s and characteristic age 0.4 Myr …

We present the results of a search for transient radio bursts of between 0.125 and 32 ms
duration in two archival pulsar surveys of intermediate Galactic latitudes with the Parkes …

We present the search methods and initial results for transient radio signals in the High Time
Resolution Universe (HTRU) survey. The HTRU survey's single-pulse search, the software …