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A Synthesis Telescope at Molonglo

  • B. Y. Mills (a1), A. G. Little (a1) and G. H. Joss (a1)

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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.

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Mills, B. Y., Aitchison, R. E., Little, A. G., and McAdam, W. B., Proc. I.R.E. (Aust.), 24, 156165, (1963).
Mills, B. Y., and Little, A. G., Proc. Ast. Soc. Aust, 2, No. 3, 134135,(1972).

A Synthesis Telescope at Molonglo

  • B. Y. Mills (a1), A. G. Little (a1) and G. H. Joss (a1)

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