Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-26T22:13:57.864Z Has data issue: false hasContentIssue false

Hazards and Future Improvements to HI Surveys

Published online by Cambridge University Press:  05 March 2013

J. Richard Fisher*
Affiliation:
National Radio Astronomy Observatory, PO Box 2, Green Bank, WV 24944, USA; [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Most radio astronomical observations are affected to some degree by man-made and natural interference. There are a few avoidance techniques that can reduce the impact of interference on the survey, but we must make quite significant advances in the understanding of our antennas and receivers and the interference itself before a substantial improvement can be expected. A major increase in the efficiency of future surveys will likely come from phased-array feeds, which have the potential for much closer beam spacings, greater antenna efficiency, and wider fields of view than current independent-feed arrays.

Type
Research Article
Copyright
Copyright © Astronomical Society of Australia 1997

References

Briggs, F. H., Sorar, E., Kraan-Korteweg, R. C., & van Driel, W. 1997, PASA, 14, 37 Google Scholar
Du Hamel, R. H., & Scherer, J. P. 1993, Frequency-independent Antennas, Ch. 14 in Antenna Engineering Handbook, 3rd edn, ed. Johnson, R. C. (New York: McGraw-Hill), 5382 Google Scholar
Gulkis, S., Olsen, E. T., Klein, M. J., & Jackson, E. B. 1991, in Light Polution, Radio Interference, and Space Debris, ASP Conf. Ser. 17, ed. Crawford, D. J. (San Francisco: ASP), 228 Google Scholar
Saini, K. S., & Bradley, R. F. 1996, NRAO Electronics Division Internal Report No. 301Google Scholar
Swarup, G., & Venkatasubramani, T. L., 1991, ASP Conf. Ser. 17, in Light Polution, Radio Interference, and Space Debris, ASP Conf. Ser. 17, ed. Crawford, D. J. (San Francisco: ASP), 190 Google Scholar
Thompson, A. R., Gergely, T. E., & Vanden Bout, P. A. 1991, Phys. Today, 44, Nov., 41Google Scholar