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    The path to visible extreme adaptive optics with MagAO-2K and MagAO-X

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    Author
    Males, Jared R. cc
    Close, Laird M. cc
    Guyon, Olivier
    Morzinski, Katie M. cc
    Hinz, Philip
    Esposito, Simone
    Pinna, Enrico
    Xompero, Marco cc
    Briguglio, Runa
    Riccardi, Armando
    Puglisi, Alfio
    Mazin, Ben
    Ireland, Michael J.
    Weinberger, Alycia
    Conrad, Al
    Kenworthy, Matthew
    Snik, Frans
    Otten, Gilles
    Jovanovic, Nemanja
    Lozi, Julien
    Show allShow less
    Affiliation
    Univ Arizona, Steward Observ
    Issue Date
    2016-07-27
    Keywords
    adaptive optics
    exoplanets
    high contrast imaging
    
    Metadata
    Show full item record
    Publisher
    SPIE-INT SOC OPTICAL ENGINEERING
    Citation
    Jared R. Males ; Laird M. Close ; Olivier Guyon ; Katie M. Morzinski ; Philip Hinz ; Simone Esposito ; Enrico Pinna ; Marco Xompero ; Runa Briguglio ; Armando Riccardi ; Alfio Puglisi ; Ben Mazin ; Michael J. Ireland ; Alycia Weinberger ; Al Conrad ; Matthew Kenworthy ; Frans Snik ; Gilles Otten ; Nemanja Jovanovic and Julien Lozi " The path to visible extreme adaptive optics with MagAO-2K and MagAO-X ", Proc. SPIE 9909, Adaptive Optics Systems V, 990952 (July 27, 2016); doi:10.1117/12.2234105; http://dx.doi.org/10.1117/12.2234105
    Journal
    ADAPTIVE OPTICS SYSTEMS V
    Rights
    © 2016 SPIE.
    Collection Information
    This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
    Abstract
    The next generation of extremely large telescopes (ELTs) have the potential to image habitable rocky planets, if suitably optimized. This will require the development of fast high order "extreme" adaptive optics systems for the ELTs. Located near the excellent site of the future GMT, the Magellan AO system (MagAO) is an ideal on-sky testbed for high contrast imaging development. Here we discuss planned upgrades to MagAO. These include improvements in WFS sampling (enabling correction of more modes) and an increase in speed to 2000 Hz, as well as an H2RG detector upgrade for the Clio infrared camera. This NSF funded project, MagAO-2K, is planned to be on-sky in November 2016 and will significantly improve the performance of MagAO at short wavelengths. Finally, we describe MagAO-X, a visible-wavelength extreme-AO "afterburner" system under development. MagAO-X will deliver Strehl ratios of over 80% in the optical and is optimized for visible light coronagraphy.
    ISSN
    0277-786X
    DOI
    10.1117/12.2234105
    Version
    Final published version
    Additional Links
    http://proceedings.spiedigitallibrary.org/proceeding.aspx?doi=10.1117/12.2234105
    ae974a485f413a2113503eed53cd6c53
    10.1117/12.2234105
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