Paper
25 October 2004 Extreme adaptive optics testbed: results and future work
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Abstract
"Extreme" adaptive optics systems are optimized for ultra-high-contrast applications, such as ground-based extrasolar planet detection. The Extreme Adaptive Optics Testbed at UC Santa Cruz is being used to investigate and develop technologies for high-contrast imaging, especially wavefront control. A simple optical design allows us to minimize wavefront error and maximize the experimentally achievable contrast before progressing to a more complex set-up. A phase shifting diffraction interferometer is used to measure wavefront errors with sub-nm precision and accuracy. We have demonstrated RMS wavefront errors of <1.3 nm and a contrast of >10-7 over a substantial region using a shaped pupil. Current work includes the installation and characterization of a 1024-actuator Micro-Electro-Mechanical-Systems (MEMS) deformable mirror, manufactured by Boston Micro-Machines, which will be used for wavefront control. In our initial experiments we can flatten the deformable mirror to 1.8-nm RMS wavefront error within a control radius of 5-13 cycles per aperture. Ultimately this testbed will be used to test all aspects of the system architecture for an extrasolar planet-finding AO system.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Julia Wilhelmsen Evans, Gary Sommargren, Lisa Poyneer, Bruce A. Macintosh, Scott Severson, Daren Dillon, Andrew I. Sheinis, Dave Palmer, N. Jeremy Kasdin, and Scot Olivier "Extreme adaptive optics testbed: results and future work", Proc. SPIE 5490, Advancements in Adaptive Optics, (25 October 2004); https://doi.org/10.1117/12.551762
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Cited by 7 scholarly publications.
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KEYWORDS
Wavefronts

Adaptive optics

Microelectromechanical systems

Diffraction

Optical testing

Point spread functions

Control systems

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