activity
20072009
most citedScience with ASKAP - the Australian Square Kilometre Array Pathfinder

414 citations · 1.1k across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.IM200924 cited

Digital Instrumentation for the Radio Astronomy Community

Aaron Parsons, Dan Werthimer, Donald Backer +21

Time-to-science is an important figure of merit for digital instrumentation serving the astronomical community. A digital signal processing (DSP) community is forming that uses sha…

astro-ph.SR2009

Precision VLBI astrometry: Instrumentation, algorithms and pulsar parallax determination

A. T. Deller

(Abridged) This thesis describes the development of DiFX, the first general-purpose software correlator for radio interferometry, and its use with the Australian Long Baseline Arra…

astro-ph2008414 cited

Science with ASKAP - the Australian Square Kilometre Array Pathfinder

S. Johnston, R. Taylor, M. Bailes +47

[ABRIDGED VERSION] The future of cm and m-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries. The SKA will be…

physics.geo-ph200812 cited

The use of the Long Baseline Array in Australia for precise geodesy and absolute astrometry

Leonid Petrov, Chris Phillips, Alessandra Bertarini +3

We report the results of a successful 12 hour 22 GHz VLBI experiment using a heterogeneous network that includes radio telescopes of the Long Baseline Array (LBA) in Australia and…

astro-ph2008124 cited

Extremely high precision VLBI astrometry of PSR J0437-4715 and implications for theories of gravity

A. T. Deller, J. P. W. Verbiest, S. J. Tingay +1

Using the recently upgraded Long Baseline Array, we have measured the trigonometric parallax of PSR J0437-4715 to better than 1% precision, the most precise pulsar distance determi…

astro-ph200733 cited

VLBI detection of an Infrared-Faint Radio Source

Ray P. Norris, Steven Tingay, Chris Phillips +3

Infrared-Faint Radio Sources represent a new and unexpected class of object which is bright at radio wavelengths but unusually faint at infrared wavelengths. If, like most mJy radi…