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17 October 1997 Adaptive optics pipeline data reduction: application to spectroimaging with Fabry-Perot
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Abstract
Adonis, the Adaptive Optics instrument on use on the ESO 3.6m telescope in la Silla, is available for the astronomical community since April 1993. Since August 1996, a Posix-compatible toolset has been installed to perform the basic steps of infra-red data preprocessing in all imaging modes, and since May 1997, the Fabry-Perot observation mode is also handled. The principles and tools of pipeline processing for adaptive optics infrared data are introduced here, together with examples for Fabry-Perot imaging reduction.
© (1997) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Nicolas Devillard, Christian Drouet D'Aubigny, and Patrice Corporon "Adaptive optics pipeline data reduction: application to spectroimaging with Fabry-Perot", Proc. SPIE 3126, Adaptive Optics and Applications, (17 October 1997); https://doi.org/10.1117/12.290160
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