Hostname: page-component-848d4c4894-xm8r8 Total loading time: 0 Render date: 2024-07-02T15:58:40.878Z Has data issue: false hasContentIssue false
  • English
  • Français

A Possible Configuration for the Australian Synthesis Telescope

Published online by Cambridge University Press:  25 April 2016

R. N. Manchester
R. N. Manchester*
Affiliation:
Division of Radiophysics, CSIRO, Sydney
Get access Rights & Permissions [Opens in a new window]

Extract

The proposal made to ASTEC for an Australian systhesis telescope (AST) is for a high-sensitivity, high-resolution synthesis array to be located at the Australian National Radio Astronomy Observatory, Parkes, and used in conjunction with the existing 64-m antenna at that site as a national facility (Wellington 1976). During the past 18 months a design study group consisting of representatives from the Australian National University, University of Sydney, University of Tasmania and CSIRO has been investigating the design of such an array. This paper reports on one aspect of this design, the array configuration.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 3 , Issue 2 , September 1977 , pp. 103 - 105
Copyright
Copyright © Astronomical Society of Australia 1977

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

Ables, J. G., Proc. Astron. Soc. Aust., 3, “Other Papers” 184 (1977).Google Scholar
Blum, E. J. Ribes, J. C., and Biraud, F., Astron. Astrophys., 41, 409 (1975).Google Scholar
Heeschen, D. S., Sky Telesc., 51, 344 (1975).Google Scholar
Wellington, K. J., Proc. Astron. Soc. Aust., 3, 7 (1976).Google Scholar