| Issue |
EAS Publications Series
Volume 69-70, 2014
What the Highest Angular Resolution Can Bring to Stellar Astrophysics?
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|
|---|---|---|
| Page(s) | 101 - 131 | |
| Section | Notions of Long-Baseline Interferometry | |
| DOI | https://doi.org/10.1051/eas/1569006 | |
| Published online | 10 September 2015 | |
What the Highest Angular Resolution Can Bring to Stellar Astrophysics?
F. Millour, A. Chiavassa, L. Bigot, O. Chesneau, A. Meilland and Ph. Stee (eds)
EAS Publications Series, 69–70 (2014) 101-131
F. Millour, A. Chiavassa, L. Bigot, O. Chesneau, A. Meilland and Ph. Stee (eds)
EAS Publications Series, 69–70 (2014) 101-131
The CLASSIC/CLIMB Data Reduction: The Software
The CHARA Array Mount Wilson Obervatory, CA 91001, USA
This is one of two chapters that describe the methods used to extract closure phase from CLIMB data and visibility amplitude from both the CLASSIC and CLIMB beam combiners. In this, the second chapter, I describe the pipeline software.
© EAS, EDP Sciences, 2015