Hostname: page-component-cd9895bd7-lnqnp Total loading time: 0 Render date: 2024-12-25T15:38:18.438Z Has data issue: false hasContentIssue false
  • English
  • Français

Radio Arrays - mm to Meters

Published online by Cambridge University Press:  19 July 2016

R.A. Perley
R.A. Perley*
Affiliation:
National Radio Astronomy Observatory, P.O. Box O, Socorro, N.M. 87801, U.S.A.

Extract

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.

There are now approximately two dozen operating interferometers in astronomy, with more under construction or in planning. The wide distribution of interferometer arrays, and their acceptance as essential tools in astronomy are a result of the remarkable flexibility and imaging capabilities of modern arrays. Much of the success of these arrays is due to advances in data processing and imaging brought about by innovative and powerful algorithms.

Type
Radio Array Instruments
Information
Symposium - International Astronomical Union , Volume 158: Very High Angular Resolution Imaging , 1994 , pp. 109 - 116
Copyright
Copyright © Kluwer 1994 

References

Christiansen, W.N. and Hogbom, J.A. 1969. Radiotelescopes, Cambridge University Press Google Scholar
Cornwell, T.J. 1993. VLA Scientific Memo 164, NRAO Google Scholar
Daishido, T. et al., 1991. in Radio Interferometry: Theory, Techniques and Applications, ASP Conference Series Vol. 19 Google Scholar
Perley, R.A. 1989 in Synthesis Imaging in Radio Astronomy, ASP Conference Series Vol 6 Google Scholar
Perley, R.A. and Cornwell, T.J. 1993. in Radio Interferometry: Theory, Techniques and Applications, ASP Conf. Series Vol 19 Google Scholar