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Radio path length correction using water vapour radiometry
R. J. Sault, G. J. Carrad, P. J. Hall +1
Path length changes through the atmosphere cause significant errors for astronomical radio interferometry at high frequencies (e.g. 100 GHz). Path length differences typically give…
Longitude-resolved imaging of Jupiter at lambda = 2 cm
R. J. Sault, C. Engel, Imke de Pater
We present a technique for creating a longitude-resolved image of Jupiter's thermal radio emission. The technique has been applied to VLA data taken on 25 January 1996 at a wavelen…
A retrospective view of Miriad
R. J. Sault, P. J. Teuben, M. C. H. Wright
Miriad is a radio interferometry data-reduction package, designed for taking raw data through to the image analysis stage. The Miriad project, begun in 1988, is now middle-aged. Wi…
The ATCA Seeing Monitor
Enno Middelberg, Robert J. Sault, Michael J. Kesteven
We present the design of, and a first analysis of data from, the atmospheric seeing monitor at the Australia Telescope Compact Array (ATCA). The seeing monitor has been operational…
1.4 GHz polarimetric observations of the two fields imaged by the DASI experiment
G. Bernardi, E. Carretti, R. J. Sault +2
We present results of polarization observations at 1.4 GHz of the two fields imaged by the DASI experiment (, and $α= 00^{\rm h} 30^{\rm…
Radio observations of the planetary nebula around the OH/IR Star OH354.88-0.54 (V1018 Sco)
Martin Cohen, Jessica M. Chapman, Rachel M. Deacon +3
We present radio observations of the unique, recently formed, planetary nebula (PN) associated with a very long-period OH/IR variable star V1018 Sco that is unequivocally still in…