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The Molonglo Catalogue Survey

Published online by Cambridge University Press:  25 April 2016

I. M. Davies
I. M. Davies*
Affiliation:
Cornell-Sydney University Astronomy Centre School of Physics, University of Sydney
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Extract

One of the basic tasks of the one-mile cross at the Molonglo Radio Observatory is the compilation of a catalogue of radio sources complete to a low flux density level. This level has been tentatively chosen as 0.2 f.u., which is well above the ultimate detection level which can be reached in selected areas of sky. Such a limitation is necessary if the catalogue is to be restricted to a manageable number of sources; a few tens of thousands, which will be achieved with the above limit, seems appropriate and useful at the present time.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 7 , April 1970 , pp. 340 - 341
Copyright
Copyright © Astronomical Society of Australia 1970

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References

1 Mills, B. Y., Aitchison, R. E., Little, A. G. and McAdam, W. B., Proc. IREE Aust., 24, 156 (1956).Google Scholar
2 Clarke, T. W., Frater, R. H., Large, M. I., Munro, R. E. B. and Murdoch, H. S., Aust. J. Phys., Astrophyskal Supplement, 10, 34 (1969).Google Scholar
3 Campbell, D. B., M.Sc. thesis, University of Sydney 1964.Google Scholar
4 Hunstead, R. W., Proc.ASA, 1, 231 (1969).Google Scholar