Hostname: page-component-cd9895bd7-gxg78 Total loading time: 0 Render date: 2024-12-27T21:44:06.953Z Has data issue: false hasContentIssue false
  • English
  • Français

Deep Surveys with the Molonglo Radio Telescope

Published online by Cambridge University Press:  25 April 2016

J. G. Robertson
J. G. Robertson*
Affiliation:
Astrophysics Department, School of Physics, University of Sydney
Get access Rights & Permissions [Opens in a new window]

Extract

Four catalogues based on the survey made with the Molonglo Cross-type radio telescope have so far been completed, the largest of which is MCI (Davies, Little and Mills,1973). These catalogues were noise limited and had a 5α lower limit of about 0.3 Jy. This paper gives an outline of deep surveys that have been made in order to reach significantly fainter sources, but only in a small solid angle of sky.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 3 , Issue 1 , September 1976 , pp. 83 - 84
Copyright
Copyright © Astronomical Society of Australia 1976

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Condon, J. J., and Jauncey, D. L., Astrophys. J. Letters, 184, L33 (1973).CrossRefGoogle Scholar
Davies, I. M., Little, A. G., and Mills, B. Y., Aust. J. Phys. Astrophys. Suppl., No. 28 (1973).Google Scholar
Jauncey, D. L., Ann. Rev. Astron. and Astrophys., 13, 23 (1975).Google Scholar
McVittie, G. C., General Relativity and Cosmology, Chapman and Hall, London (1965).Google Scholar
Pearson, T. Mon. Not. R. Astro. Soc., 171, 475 (1975).Google Scholar
Robertson, J. G., Aust. J. Phys., 26, 403 (1973).Google Scholar
Sutton, J. M., Davies, I. M., Little, A. G., and Murdoch, H. S., Aust.J. Phys. Astrophys. Suppl, No. 33 (1974).Google Scholar