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A Summary of Recent Observations with the Parkes Interferometer

Published online by Cambridge University Press:  25 April 2016

J.V. Wall ,
D.J. Cole  and
D.K. Milne
J.V. Wall
Affiliation:
Mount Stromlo Observatory, Australian National University, Canberra
D.J. Cole
Affiliation:
Division of Radiophysics, CSIRO, Sydney
D.K. Milne
Affiliation:
Division of Radiophysics, CSIRO, Sydney
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Extract

The Parkes interferometer consists of the 210-ft para-boloidal reflector of the ANRAO, and a 60-ft paraboloidal reflector mounted on rail tracks. These extend from 400 ft to 1400 ft from the 210-ft paraboloid and run both north-south and east-west. The baseline may be continuously varied during observation; receivers operating simultaneously at 468 and 1402 MHz enable the determination of complete visibility functions over the range 200λ to 2000λ.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 3 , February 1968 , pp. 98
Copyright
Copyright © Astronomical Society of Australia 1968

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References

1 Cole, D.L., Proc. ASA, 1, 30 (1967).Google Scholar
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4 Fomalont, E.B., Ph.D. thesis, California Institute of Technology, 1967.Google Scholar
5 Bolton, J.G., and Kinman, T.D. Astrophys. J., 145, 951 (1966).Google Scholar
6 Westerlund, B.E., private communication.Google Scholar
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8 McVittie, G.C., Astrophys. J., 142, 1637 (1965).CrossRefGoogle Scholar