Paper
28 June 2006 The extreme adaptive optics testbed at UCSC: current results and coronagraphic upgrade
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Abstract
We present a summary of our current results from the Extreme Adaptive Optics (ExAO) Testbed and the design and status of its coronagraphic upgrade. The ExAO Testbed at the Laboratory for Adaptive Optics at UCO/Lick Observatory is optimized for ultra-high contrast applications requiring high-order wavefront control. It is being used to investigate and develop technologies for the Gemini Planet Imager (GPI). The testbed is equipped with a phase shifting diffraction interferometer (PSDI), which measures the wavefront with sub-nm precision and accuracy. The testbed also includes a 1024-actuator Micro Electro Mechanical Systems (MEMS) deformable mirror manufactured by Boston Micromachines. We present a summary of the current results with the testbed encompassing MEMS flattening via PSDI, MEMS flattening via a Shack-Hartmann wavefront sensor (with and without spatial filtering), the introduction of Kolmogorov phase screens, and contrast in the far-field. Upgrades in progress include adding additional focal and pupil planes to better control scattered light and allow alternative coronagraph architectures, the introduction and testing of high-quality reflecting optics, and a variety of input phase aberrations. Ultimately, the system will serve as a full prototype for GPI.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Scott A. Severson, Brian Bauman, Daren Dillon, Julia Evans, Don Gavel, Bruce Macintosh, Katie Morzinski, Dave Palmer, and Lisa Poyneer "The extreme adaptive optics testbed at UCSC: current results and coronagraphic upgrade", Proc. SPIE 6272, Advances in Adaptive Optics II, 62722J (28 June 2006); https://doi.org/10.1117/12.672341
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Cited by 10 scholarly publications.
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KEYWORDS
Wavefronts

Microelectromechanical systems

Actuators

Coronagraphy

Adaptive optics

Gemini Planet Imager

Wavefront sensors

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