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A Synthesis Telescope at Molonglo

Published online by Cambridge University Press:  25 April 2016

B. Y. Mills ,
A. G. Little  and
G. H. Joss
B. Y. Mills
Affiliation:
School of Physics, University of Sydney
A. G. Little
Affiliation:
School of Physics, University of Sydney
G. H. Joss
Affiliation:
School of Physics, University of Sydney
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Extract

The major programs at the Molonglo Radio Observatory are nearing completion. Much can still be done using the existing 1 mile Cross-type radio-telescope (Mills et al. 1963) but, to tackle properly many of the current problems in radio astronomy, a fundamental change is required from a transit to a trackable radio-telescope, combined with an increase in the operating frequency and the resolution.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 3 , Issue 1 , September 1976 , pp. 33 - 34
Copyright
Copyright © Astronomical Society of Australia 1976

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References

Mills, B. Y., Aitchison, R. E., Little, A. G., and McAdam, W. B., Proc. I.R.E. (Aust.), 24, 156–165, (1963).Google Scholar
Mills, B. Y., and Little, A. G., Proc. Ast. Soc. Aust, 2, No. 3, 134–135,(1972).Google Scholar