Although fifty years have passed since the discovery of radio pulsars, there is still no
satisfactory understanding of how these amazing objects operate. While there has been …

We present a study of the spectral properties of 441 pulsars observed with the Parkes radio
telescope near the centre frequencies of 728, 1382 and 3100 MHz. The observations at 728 …

We describe a new low-frequency wideband radio survey of the southern sky. Observations
covering 72–231 MHz and Declinations south of have been performed with the Murchison …

The radio spectral index is a powerful probe for classifying cosmic radio sources and
understanding the origin of the radio emission. Combining data at 147 MHz and 1.4 GHz …

We present results from the first all-sky radio survey in circular polarization. The survey uses
the Murchison Widefield Array (MWA) to cover 30 900 sq deg, over declinations south of+ …

We present the results of a coordinated campaign conducted with the Murchison Widefield
Array (MWA) to shadow fast radio bursts (FRBs) detected by the Australian Square Kilometre …

We present techniques developed to calibrate and correct Murchison Widefield Array low-
frequency (72–300 MHz) radio observations for polarimetry. The extremely wide field-of …

The Murchison Widefield Array (MWA) is an open access telescope dedicated to studying
the low-frequency (80–300 MHz) southern sky. Since beginning operations in mid-2013, the …

Abstract The Green Bank North Celestial Cap (GBNCC) pulsar survey will cover the entire
northern sky (δ>− 40) at 350 MHz, and is one of the most uniform and sensitive all-sky pulsar …

We present the detection of 661 known pulsars observed with the Australian SKA Pathfinder
(ASKAP) telescope at 888 MHz as part of the Rapid ASKAP Continuum Survey (RACS) …