Proceedings ArticleDOI
The extreme adaptive optics testbed at UCSC: current results and coronagraphic upgrade
Scott Severson,Brian J. Bauman,Daren Dillon,Julia W. Evans,Donald T. Gavel,Bruce Macintosh,Katie M. Morzinski,Dave Palmer,Lisa Poyneer +8 more
TLDR
The Extreme Adaptive Optics (ExAO) Testbed at UCO/Lick is optimized for ultra-high contrast applications requiring high-order wavefront control as discussed by the authors.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.read more
Citations
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Proceedings ArticleDOI
The open-loop control of MEMS: modeling and experimental results
Katie M. Morzinski,Katie M. Morzinski,Kennet B. W. Harpsøe,Kennet B. W. Harpsøe,Donald T. Gavel,Donald T. Gavel,S. Mark Ammons,S. Mark Ammons +7 more
TL;DR: In this article, the authors present a formulation for accurate open-loop control of MEMS deformable mirrors, which can be used for wide field and high-order wavefront correction systems.
Journal ArticleDOI
Correction of Non–Common-Path Error for Extreme Adaptive Optics
TL;DR: In this paper, the authors proposed a simple approach that can be used to eliminate differential aberration with extreme adaptive optics and is optimized for best image performance or directly optimized for high-contrast coronagraphic imaging.
Proceedings ArticleDOI
Preliminary characterization of Boston Micromachines' 4096-actuator deformable mirror
Andrew Norton,Julia Wilhelmson Evans,Donald T. Gavel,Daren Dillon,David Palmer,Bruce Macintosh,Katie M. Morzinski,Steven Cornelissen +7 more
TL;DR: In this paper, the performance of Boston Micromachine 4096-actuator deformable mirror (DM) was evaluated for the Gemini Planet Imager high-contrast adaptive optics (AO) system.
Journal ArticleDOI
Stroke saturation on a MEMS deformable mirror for woofer-tweeter adaptive optics.
TL;DR: High-contrast imaging of extrasolar planet candidates around a main-sequence star has recently been realized from the ground using current adaptive optics (AO) systems, implying that correlations through the influence functions are important.
Proceedings ArticleDOI
Shaping light: MOEMS deformable mirrors for microscopes and telescopes
TL;DR: In this article, the authors describe their efforts at Boston University and at Boston Micromachines Corporation to design, fabricate, and control MOEMS DMs for adaptive optics (AO) applications.
References
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A Nongray Theory of Extrasolar Giant Planets and Brown Dwarfs
Adam Burrows,Mark S. Marley,William B. Hubbard,Jonathan I. Lunine,Tristan Guillot,Didier Saumon,Richard S. Freedman,David Sudarsky,C. M. Sharp +8 more
TL;DR: In this article, the authors present a series of nongray calculations of the atmospheres, spectra, colors, and evolution of extrasolar giant planets (EGPs) and brown dwarfs for effective temperatures below 1300 K.
Proceedings ArticleDOI
The Gemini Planet Imager
Bruce Macintosh,James R. Graham,David Palmer,René Doyon,Donald T. Gavel,James E. Larkin,Ben R. Oppenheimer,L. Saddlemyer,J. Kent Wallace,Brian J. Bauman,Julia W. Evans,Darren Erikson,Katie M. Morzinski,Donald W. Phillion,Lisa Poyneer,Anand Sivaramakrishnan,Rémi Soummer,Simon Thibault,Jean-Pierre Véran +18 more
TL;DR: The Gemini Planet Imager (GPI) as discussed by the authors is a system for direct imaging of the planets themselves, which can achieve contrast levels of 10-7 to 10-8, sufficient to detect warm self-luminous Jovian planets.
Journal ArticleDOI
Speckle Decorrelation and Dynamic Range in Speckle Noise-limited Imaging
TL;DR: In this article, it was shown that the original speckles must persist and that the technique of speckle decorrelation merely adds more noise to the original noise, thereby degrading the dynamic range of the image.
Journal ArticleDOI
Optimal modal Fourier-transform wavefront control
Lisa Poyneer,Jean-Pierre Véran +1 more
TL;DR: The modal basis is the real Fourier basis, which allows direct control of specific regions of the point-spread function and is computationally efficient enough to be implemented with off-the-shelf technology for a 2.5 kHz, 64 x 64 adaptive optics system.
Journal ArticleDOI
What Fraction of Sun-like Stars have Planets?
TL;DR: In this article, the radial velocities of ~1800 nearby Sun-like stars are currently being monitored by eight high-sensitivity Doppler exoplanet surveys, and the authors find that at least 9% of these stars have planets in the mass and orbital period ranges M sin i > 0.3MJup and P 0.1MJup.
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The Gemini Planet Imager
Bruce Macintosh,James R. Graham,David Palmer,René Doyon,Donald T. Gavel,James E. Larkin,Ben R. Oppenheimer,L. Saddlemyer,J. Kent Wallace,Brian J. Bauman,Julia W. Evans,Darren Erikson,Katie M. Morzinski,Donald W. Phillion,Lisa Poyneer,Anand Sivaramakrishnan,Rémi Soummer,Simon Thibault,Jean-Pierre Véran +18 more