Paper
12 July 2008 The SPHERE XAO system: design and performance
Author Affiliations +
Abstract
Extreme adaptive optics system (SAXO) is the heart of the SPHERE instrument which aims at directly detect and characterize giant extra-solar planets from the ground. It should equip one of the four VLT 8-m telescopes at the end of 2010. We present a detailed design and architecture of the SAXO system. We focus on each critical point that has been solved during the preliminary design phase. It concerns the adaptive optics system itself but also the interaction with other SPHERE subsystems (such as coronagraphy) and focal plane instrumentation (dual band imager, integral field spectroscopy and polarimetric imager). Acceptance and integration tests of SAXO are discussed. Finally, detailed performance of the whole system and comparison to the science requirements are provided.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Cyril Petit, Thierry Fusco, Julien Charton, David Mouillet, Patrick Rabou, Tristan Buey, Gérard Rousset, Jean-François Sauvage, Pierre Baudoz, Pierre Gigan, Markus Kasper, Enrico Fedrigo, Norbert Hubin, Philippe Feautrier, Jean-Luc Beuzit, and Pascal Puget "The SPHERE XAO system: design and performance", Proc. SPIE 7015, Adaptive Optics Systems, 70151U (12 July 2008); https://doi.org/10.1117/12.790308
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Cited by 18 scholarly publications.
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KEYWORDS
Adaptive optics

Coronagraphy

Optical spheres

Calibration

Sensors

Imaging systems

Stars

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