Pulsar dispersion measures (DMs) have been used to model the electron density of the
interstellar medium (ISM) in the Galactic disk as a plane-parallel medium, despite significant …

We present initial pulsar results from the first station of the Long Wavelength Array (LWA1)
obtained during the commissioning period of LWA1 and in early science results. We present …

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 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 …

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 …

In this paper the anomalous intense pulse of PSR J0953+ 0755 was studied in the
decametre wavelength range. For this pulse, two scales of fine structure were discovered …

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 present the results of the simultaneous observation of giant radio pulses (GRPs) from the
Crab pulsar at 0.3, 1.6, 2.2, 6.7, and 8.4 GHz with four telescopes in Japan. We obtain 3194 …

ABSTRACT With the Expanded Long Wavelength Array and pulsar binning techniques, we
searched for off-pulse emission from PSR B0950+ 08 at 76 MHz. Previous studies suggest …