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

PSR B0950+ 08 is a bright nonrecycled pulsar whose single-pulse fluence variability is
reportedly large. Based on observations at two widely separated frequencies, 55 MHz …

We present the first Southern-Hemisphere all-sky imager and radio-transient monitoring
system implemented on two prototype stations of the low-frequency component of the …

We report on simultaneous wideband observations of Crab giant pulses with the Parkes
radio telescope and the Murchison Widefield Array (MWA). The observations were …

Abstract We present 154 MHz Murchison Widefield Array imaging observations and
variability information for a sample of pulsars. Over the declination range− 80°< δ< 10°, we …

Abstract Rotating Radio Transients are a relatively new subclass of pulsar characterized by
sporadic bursting emission of single pulses. Here, we present a single-pulse analysis of a …

We report on the detection of extreme giant pulses (GPs) from one of the oldest known
pulsars, the highly variable PSR B0950+ 08, with the Amsterdam-ASTRON Radio Transient …

We report the emission variations in PSR J1047− 6709 observed at 1369 MHz using the
Parkes 64-m radio telescope. This pulsar shows two distinct emission states: a weak state …

Pulsars are known as the 'lighthouses' of the Universe. Periodic pulses with a duty cycle of
are detected when the radio beam of a rotating pulsar sweeps across the telescope. In this …

We report the detection of giant pulse (GP) emission from PSR B0950+ 08 in 24 hours of
observations made at 39.4 MHz, with a bandwidth of 16 MHz, using the first station of the …