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The Molonglo Radio Source Surveys at 408 MHz

Published online by Cambridge University Press:  14 August 2015

B. Y. Mills
B. Y. Mills*
Affiliation:
School of Physics, University of Sydney, Australia.

Extract

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One of the basic programs undertaken with the 1 mile Cross-type radio telescope at the Molonglo Radio Observatory has been a systematic survey of the sky south of +18° declination. Commencing in late 1967, the survey has been continuing at a low priority until it is now complete to a declination of −85°, except for some small areas affected by interference or instrumental problems which are being re-observed. A program of ‘deep surveys’ is also being undertaken; this involves multiple observations within narrow strips at selected declinations. The signal-to-noise ratio is some three to five times better than in normal surveying and the confusion limit is approached.

Type
I. Surveys of Radio Sources, Source Counts and Anisotropies
Information
Symposium - International Astronomical Union , Volume 74: Radio Astronomy and Cosmology , 1977 , pp. 31 - 37
Copyright
Copyright © Reidel 1977 

References

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