Previous | Session 153 | Next
P. R. Lawson (JPL), W. D. Cotton (NRAO), C. A. Hummel (ESO), J. D. Monnier, M. Zhao (Univ. Michigan), J. S. Young, H. Thorsteinsson (Univ. Cambridge), S. C. Meimon, L. Mugnier, G. Le Besnerais (ONERA), E. Thiebaut (Observatoire de Lyon), P. G. Tuthill (Univ. Sydney)
We present a formal comparison of the performance of algorithms used for synthesis imaging with optical/infrared long-baseline interferometers. Five different algorithms are evaluated based on their performance with simulated test data. The strengths and limitations of each algorithm are discussed.
If you would like more information about this abstract, please follow the link to http://olbin.jpl.nasa.gov/iau/2004/beauty.html. This link was provided by the author. When you follow it, you will leave the Web site for this meeting; to return, you should use the Back comand on your browser.
The author(s) of this abstract have provided an email address for comments about the abstract: Peter.Lawson@jpl.nasa.gov
Previous | Session 153 | Next
Bulletin of the American Astronomical Society, 36 5
© 2004. The American Astronomical Society.