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.
Original language | English |
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Title of host publication | Advances in Stellar Interferometry |
Place of Publication | Bellingham, Wash. |
Publisher | SPIE |
Pages | 1-12 |
Number of pages | 12 |
Volume | 6268 I |
ISBN (Print) | 0819463337, 9780819463333 |
DOIs | |
Publication status | Published - 2006 |
Externally published | Yes |
Event | Advances in Stellar Interferometry - Orlando, FL, United States Duration: 25 May 2006 → 30 May 2006 |
Other
Other | Advances in Stellar Interferometry |
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Country/Territory | United States |
City | Orlando, FL |
Period | 25/05/06 → 30/05/06 |
Keywords
- Aperture synthesis
- Astronomical software
- Closure phase
- Imaging
- Infrared
- Interferometry
- Optical