Two years of pulsar observations with the Ultra-Wideband Receiver on the Parkes radio telescope
Simon Johnston,
C. Sobey,
S. Dai
et al.
Abstract:The major programme for observing young, non-recycled pulsars with the Parkes telescope has transitioned from a narrow-band system to an ultra-wideband system capable of observing between 704 and 4032 MHz. We report here on the initial two years of observations with this receiver. Results include dispersion measure (DM) and Faraday rotation measure (RM) variability with time, determined with higher precision than hitherto, flux density measurements and the discovery of several nulling and mode changing pulsars… Show more
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