Hostname: page-component-8448b6f56d-wq2xx Total loading time: 0 Render date: 2024-04-18T23:03:46.268Z Has data issue: false hasContentIssue false

High resolution mapping with the FST

Published online by Cambridge University Press:  25 April 2016

J . D. Bunton
Affiliation:
School of Electrical Engineering, University of Sydney
I. G. Jones
Affiliation:
School of Electrical Engineering, University of Sydney
D. R. Brown
Affiliation:
School of Electrical Engineering, University of Sydney

Abstract

Recent modifications to the Fleurs digital receiver enable the additional correlations between the six 13.7 m dishes to be measured. Previously, only those correlations formed between the four east-west 13.7 m dishes and the thirty-two 5.7 m dishes were measured. This enables the production of three type of maps; each with full 20 arc second resolution but with properties which suit differing astronomical applications.

Type
Contributions
Copyright
Copyright © Astronomical Society of Australia 1985

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

Bracewell, R. N., 1983, Indirect Imaging, ed. Roberts, J. A., page 117, Cambridge University Press.Google Scholar
Christiansen, W. N., 1973, Proc. IREE, 34, 302.Google Scholar
Frater, R. H., 1978, Astron. Astrophys., 68, 397.Google Scholar
Goss, W. M., and Shaver, P. A., 1970, Aust. J. Phys. Astrophys. Suppl., 14, 1.Google Scholar
Jones, I. G., Watkinson, A., Egau, P. C., Percival, T. M., Skellern, D. J., and Graves, G. R., 1984, Proc. Astron. Soc. Aust., 5, 574.CrossRefGoogle Scholar
Shaver, P. A., and Goss, W. M., 1970, Aust. J. Phys. Astrophys. Suppl., 14, 77.Google Scholar