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22 GHz Observations with the Resurfaced Central 17 m of the Parkes Radio Telescope

Published online by Cambridge University Press:  25 April 2016

J. L. Caswell ,
R. A. Batchelor ,
W. M. Goss ,
R. F. Haynes ,
S. H. Knowles ,
K. J. Wellington ,
D. E. Yabsley  and
M. Balister
J. L. Caswell
Affiliation:
Division of Radiophysics, CSIRO, Sydney
R. A. Batchelor
Affiliation:
Division of Radiophysics, CSIRO, Sydney
W. M. Goss
Affiliation:
Division of Radiophysics, CSIRO, Sydney
R. F. Haynes
Affiliation:
Division of Radiophysics, CSIRO, Sydney
S. H. Knowles
Affiliation:
Division of Radiophysics, CSIRO, Sydney
K. J. Wellington
Affiliation:
Division of Radiophysics, CSIRO, Sydney
D. E. Yabsley
Affiliation:
Division of Radiophysics, CSIRO, Sydney
M. Balister
Affiliation:
Division of Radiophysics, CSIRO, Sydney
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Extract

At the centre of the Parkes 64—m radio telescope a region of diameter 17 m has recently been resurfaced to improve its efficiency at high frequencies. The first measurements using this section have been made at 22 GHz, in observations of both continuum sources and water tfapour masers. For these observations the receiver front-end used a mixer cooled in liquid nitrogen, followed by a 5 GHz cryogenic parametric amplifier as a second stage. The option of switching against an offset horn was available and the total systemnoise temperature was ∽ 750 K.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 3 , Issue 1 , September 1976 , pp. 61 - 63
Copyright
Copyright © Astronomical Society of Australia 1976

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References

Caswell, J. L., Batchelor, R. A., Haynes, R. F., and Huchtmeier, W. K., Aust. J. Phys., 21, All (1974).Google Scholar
Cato, B. T., Romnang, B. O., Lewin, P. T., Rydbeck, O. E. H., Yngvesson, K. S., Cardiasnos, A. G., and Shanley, J. F., Res. Rep. No. 123, Research Laboratory of Electronics and Onsala Space Observatory, Chalmers University of Technology, Gothenburg (1975).Google Scholar
Hills, R., Janssen, M. A., Thornton, D. D., and Welch, W. J., Astrophys. J., 175, L59 (1972).Google Scholar
Johnston, K. J., Sloanaker, R. M., and Bologna, J. M., Astrophys. J., 182, 67 (1973).Google Scholar
Johnston, K. J., Robinson, B. J., Caswell, J. L., and Batchelor, R. A., Astrophys. Lett., 10, 93 (1972).Google Scholar
Lada, C. J., Dickinson, D. F., Gottlieb, C. A., and Wright, E. L., Astrophys. J., (in press) (1976).Google Scholar
Turner, B. E., and Rubin, R. H., Astrophys. J., 170, L113 (1971).Google Scholar