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The Synthesised Beamshapes for the Fleurs Extension

Published online by Cambridge University Press:  25 April 2016

R. H. Frater ,
R. G. Gough  and
A. Watkinson
R. H. Frater
Affiliation:
School of Electrical Engineering, University of Sydney
R. G. Gough
Affiliation:
School of Electrical Engineering, University of Sydney
A. Watkinson
Affiliation:
School of Electrical Engineering, University of Sydney
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Extract

A proposal for the siting of additional 14 metre antennas for the Fleurs Synthesis Telescope (FST) was previously presented by Christiansen (1976). Since that time, difficulties have arisen which preclude the use of two of the locations. In addition, solutions to the problems of data reduction for irregular antenna spacings have been found (Frater and Skellern, 1978; Frater, 1978; Frater, 1979). It has now been possible to choose the locations of the final antennas to optimise the performance of the array within broader geographic constraints — subject now to the availability of sites on ‘friendly’ land.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 4 , Issue 1 , 1980 , pp. 24 - 25
Copyright
Copyright © Astronomical Society of Australia 1980

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References

Christiansen, W. N., Proc. Astron. Soc.., 3, 35 (1976).CrossRefGoogle Scholar
Frater, R. H., and Skellern, D. J., Astron. Astrophys., 68, 391 (1978).Google Scholar
Frater, R. H., Astron. Astrophys., 68, 397 (1978).Google Scholar
Frater, R. H., ‘Image Formation from Coherence Functions in Astronomy’, ed. Schooneveld, C. van, Reidel, , pp. 19–26 (1979).CrossRefGoogle Scholar