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Results from the PALM-3000 high-order adaptive optics system

Roberts, Jennifer E. and Dekany, Richard G. and Burruss, Rick S. and Baranec, Christoph and Bouchez, Antonin and Croner, Ernest E. and Guiwits, Stephen R. and Hale, David D. S. and Henning, John R. and Palmer, Dean L. and Troy, Mitchell and Truong, Tuan N. and Zolkower, Jeffry (2012) Results from the PALM-3000 high-order adaptive optics system. In: Adaptive Optics Systems III. Proceedings of SPIE. No.8447. Society of Photo-Optical Instrumentation Engineers , Bellingham, WA, Art. No. 84470Y. ISBN 9780819491480. https://resolver.caltech.edu/CaltechAUTHORS:20161025-095637834

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Abstract

The first of a new generation of high actuator density AO systems developed for large telescopes, PALM-3000 is optimized for high-contrast exoplanet science but will support operation with natural guide stars as faint as V ~ 18. PALM-3000 began commissioning in June 2011 on the Palomar 200" telescope and has to date over 60 nights of observing. The AO system consists of two Xinetics deformable mirrors, one with 66 by 66 actuators and another with 21 by 21 actuators, a Shack-Hartman WFS with four pupil sampling modes (ranging from 64 to 8 samples across the pupil), and a full vector matrix multiply real-time system capable of running at 2KHz frame rates. We present the details of the completed system, and initial results. Operating at 2 kHz with 8.3cm pupil sampling on-sky, we have achieved a K-band Strehl ratio as high as 84% in ~1.0 arcsecond visible seeing.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1117/12.926477DOIArticle
http://proceedings.spiedigitallibrary.org/proceeding.aspx?articleid=1358894PublisherArticle
ORCID:
AuthorORCID
Baranec, Christoph0000-0002-1917-9157
Additional Information:© 2012 SPIE. This research was carried out in part at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise, does not constitute or imply its endorsement by the United States Government or the Jet Propulsion Laboratory, California Institute of Technology. This work was also supported by National Science Foundation grant AST-0619922, PI: Dr. R. Dekany. Support for the wavefront reconstructor computer has been provided by the Air Force Office of Sponsored Research, Award #FA9550-06-1-0343 (DURIP FY06). Support for the PALM-3000 3388 actuator DM was provided by a NASA Small Business Innovation Research grant #NNG06CA21C.
Funders:
Funding AgencyGrant Number
NASA/JPL/CaltechUNSPECIFIED
NSFAST-0619922
Air Force Office of Sponsored Research (AFOSR)FA9550-06-1-0343
NASANNG06CA21C
Subject Keywords:Adaptive Optics, Palomar, PALM-3000
Series Name:Proceedings of SPIE
Issue or Number:8447
Record Number:CaltechAUTHORS:20161025-095637834
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20161025-095637834
Official Citation:Jennifer E. Roberts ; Richard G. Dekany ; Rick S. Burruss ; Christoph Baranec ; Antonin Bouchez ; Ernest E. Croner ; Stephen R. Guiwits ; David D. S. Hale ; John R. Henning ; Dean L. Palmer ; Mitchell Troy ; Tuan N. Truong ; Jeffry Zolkower; Results from the PALM-3000 high-order adaptive optics system. Proc. SPIE 8447, Adaptive Optics Systems III, 84470Y (September 13, 2012); doi:10.1117/12.926477
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:71441
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:25 Oct 2016 17:31
Last Modified:03 Oct 2019 16:07

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