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The Australian experience with the PC-EVN recorder
R. Dodson, S. Tingay, C. West +4
We report on our experiences using the Metsahovi Radio Observatory's (MRO) VLBI Standard Interface (VSI, Whitney 2002) recorder in a number of astronomical applications. The PC-EVN…
COSMIC : Microarcsecond resolution with a 30 metre radio telescope
P. M. McCulloch, S. P. Ellingsen, D. L. Jauncey +4
Interstellar scintillation has been conclusively demonstrated to be the principal cause of the intraday variability (IDV) observed in the centimetre-wavelength emission of many AGN…
The Vela pulsar, the key?
Richard Dodson, Dion Lewis, David Legge +4
Of all pulsars known Vela has been one of the most productive in terms in understanding pulsars and their characteristics. We present the latest results derived from Australian tel…
Measurement of the proper motion of Vela with the LBA
Richard Dodson, David Legge, Peter McCulloch +1
The first accurate measurements of Vela's proper motion were produced using the Parkes-Tidbinbilla Interferometer (PTI) (Bailes et al 1989). This 275 km baseline at 1.6 GHz gave a…
The VSOP 2 mission: Imaging capabilities
R. Dodson, H. Hirabayashi, Y. Murata +4
Given the scientific goals of VSOP-2, including the possibility of observations of the shadows of black holes, we have investigated the fidelity of the recovered images given a typ…
The VSOP 5 GHz Continuum Survey, recent results
R. Dodson, H. Hirabayashi, P. G. Edwards +5
In February 1997 the Japanese radio astronomy satellite Halca was launched to provide the space-bourne element for the VSOP mission. Approximately twenty-five percent of the missio…