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Radio and Optical Spectra of Sources from the Molonglo Deep Survey

Published online by Cambridge University Press:  25 April 2016

H. S. Murdoch  and
G. L. White
H. S. Murdoch
Affiliation:
School of Physics, University of Sydney
G. L. White
Affiliation:
School of Physics, University of Sydney
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Extract

We present here preliminary results of further radio and optical work being carried out on the Molonglo Deep Survey (Robertson 1977a, b, c) which reaches a density of ∼ 20,000 sources per sterad at a limiting flux density of 84 mJy at 408 MHz in three small areas of sky at declinations -20° and -62°. The position errors range from 4 to 15 arc sec r.m.s. depending on flux density. Optical identifications are being made by G. W. using the Palomar Sky Survey in the -20° region and the ESO and SRC surveys in the -62° region. In the latter case, where only one colour is available more accurate positions are necessary to identify QSO candidates. The Fleurs synthesis telescope is being used to obtain accurate positions.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 3 , Issue 2 , September 1977 , pp. 142 - 143
Copyright
Copyright © Astronomical Society of Australia 1977

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References

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