dc.contributor.author |
Lawson, Peter R. |
|
dc.contributor.author |
Cotton, William D. |
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dc.contributor.author |
Hummel, Christian A. |
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dc.contributor.author |
Ireland, Michael |
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dc.contributor.author |
Monnier, John D. |
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dc.contributor.author |
Thiébaut, Eric |
|
dc.contributor.author |
Rengaswamy, Sridharan |
|
dc.contributor.author |
Baron, Fabien |
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dc.contributor.author |
Young, John S. |
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dc.contributor.author |
Kraus, Stefan |
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dc.contributor.author |
Hoffman, Karl-Heinz |
|
dc.contributor.author |
Weigelt, Gerd P. |
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dc.contributor.author |
Chesneau, Olivier |
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dc.date.accessioned |
2006-10-05T22:16:03Z |
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dc.date.available |
2006-10-05T22:16:03Z |
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dc.date.issued |
2006-05-24 |
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dc.identifier.citation |
SPIE Astronomical Telescopes and Instrumentation, Orlando, Florida, May 24-31, 2006. |
en |
dc.identifier.clearanceno |
06-1626 |
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dc.identifier.uri |
http://hdl.handle.net/2014/39822 |
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dc.description.abstract |
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. Each set of test data is formatted in the OI-FITS format. The data are calibrated power spectra and
bispectra measured with an array intended to be typical of existing imaging interferometers. The strengths and limitations of each algorithm are discussed. |
en |
dc.description.sponsorship |
NASA/JPL |
en |
dc.format.extent |
1274788 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en_US |
en |
dc.publisher |
Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2006. |
en |
dc.subject |
astronomical software |
en |
dc.subject |
interferometry |
en |
dc.subject |
closure phase |
en |
dc.subject |
aperture synthesis |
en |
dc.subject |
imaging |
en |
dc.subject |
opticals |
en |
dc.subject |
infrared |
en |
dc.title |
2006 interferometry imaging beauty contest |
en |
dc.type |
Preprint |
en |