R
Richard Dodson
Researcher at University of Western Australia
Publications - 200
Citations - 5990
Richard Dodson is an academic researcher from University of Western Australia. The author has contributed to research in topics: Very-long-baseline interferometry & Pulsar. The author has an hindex of 42, co-authored 199 publications receiving 5320 citations. Previous affiliations of Richard Dodson include University of Tasmania & Korea Astronomy and Space Science Institute.
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Science with ASKAP - the Australian Square Kilometre Array Pathfinder
Simon Johnston,R. Taylor,Matthew Bailes,Norbert Bartel,Carlton M. Baugh,Michael Bietenholz,Chris Blake,Robert Braun,Jo-Anne Brown,Shami Chatterjee,Jeremy Darling,Adam T. Deller,Richard Dodson,Philip G. Edwards,Ronald D. Ekers,Simon Ellingsen,Ilana Feain,Bryan Gaensler,Marijke Haverkorn,George Hobbs,Andrew M. Hopkins,C. A. Jackson,C. W. James,G. Joncas,V. M. Kaspi,Virginia A. Kilborn,Baerbel Koribalski,Roland Kothes,T. L. Landecker,A. Lenc,James E. J. Lovell,Jean-Pierre Macquart,Richard N. Manchester,Deanna Matthews,Naomi McClure-Griffiths,Ray P. Norris,Ue-Li Pen,Chris Phillips,Chris Power,R. J. Protheroe,Elaine M. Sadler,Brian P. Schmidt,Ingrid H. Stairs,Lister Staveley-Smith,J. M. Stil,Steven Tingay,Anastasios Tzioumis,Mark Walker,Jasper Wall,M. Wolleben +49 more
TL;DR: The Australian SKA Pathfinder (ASKAP) as discussed by the authors is aimed squarely in this frequency range, and achieves instantaneous wide-area imaging through the development and deployment of phase-array feed systems on parabolic reflectors.
Posted Content
Pulsar glitch substructure and pulsar interiors
TL;DR: Kerastari et al. as discussed by the authors found that the spin up for the Vela pulsar occurs instantaneously to within the uncertainties of the data, and the potential for new, higher resolution data, to unveil insights of the Neutron Star interiors is discussed.
Journal ArticleDOI
Small glitches and other rotational irregularities of the Vela pulsar.
Cristobal M. Espinoza,D. Antonopoulou,D. Antonopoulou,Richard Dodson,Marina Stepanova,A. Scherer +5 more
TL;DR: In this paper, the authors explore the population of small-amplitude rotational changes in the Vela pulsar and determine the rate of occurrence and sizes of its smallest glitches.
Correlations Between X-ray and Radio Pulses in Vela
Jennifer L. Donovan,Andrea N. Lommen,Zaven Arzoumanian,Alice K. Harding,M. S. Strickman,Carl R. Gwinn,Richard Dodson,P. M. McCulloch,D. Moffett +8 more
TL;DR: In this article, the authors found that Vela emits significantly more X-rays during radio pulses with strong flux than during weak radio flux pulses, which indicates that the mechanisms creating the Vela pulsar's X-ray and radio emission must be related.