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    Adaptive optics capabilities at the Large Binocular Telescope Observatory

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    Author
    Christou, J. C.
    Brusa, G.
    Conrad, A.
    Esposito, S.
    Herbst, T.
    Hinz, P.
    Hill, J. M.
    Miller, D. L.
    Rabien, S.
    Rahmer, G.
    Taylor, G. E.
    Veillet, C.
    Zhang, X.
    Show allShow less
    Affiliation
    Univ Arizona, Steward Observ
    Issue Date
    2016-07-26
    Keywords
    Natural Guide Star
    Laser Guide Star
    Adaptive Optics
    Interferometry
    Single Conjugate Adaptive Optics
    Ground Layer Adaptive Optics
    Multiple Conjugate Adaptive Optics
    Laser Guide Stars
    NIR
    MIR Extreme Adaptive Optics
    
    Metadata
    Show full item record
    Publisher
    SPIE-INT SOC OPTICAL ENGINEERING
    Citation
    J. C. Christou ; G. Brusa ; A. Conrad ; S. Esposito ; T. Herbst ; P. Hinz ; J. M. Hill ; D. L. Miller ; S. Rabien ; G. Rahmer ; G. E. Taylor ; C. Veillet and X. Zhang " Adaptive optics capabilities at the Large Binocular Telescope Observatory ", Proc. SPIE 9909, Adaptive Optics Systems V, 99092E (July 26, 2016); doi:10.1117/12.2231783; http://dx.doi.org/10.1117/12.2231783
    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
    We present an overview of the current and future adaptive optics systems at the LBTO along with the current and planned science instruments they feed. All the AO systems make use of the two 672 actuator adaptive secondary mirrors. They are (1) FLAO (NGS/SCAO) feeding the LUCI NIR imagers/spectrographs; (2) LBTI/AO (NGS/SCAO) feeding the NIR/MIR imagers and LBTI beam combiner; (3) the ARGOS LGS GLAO system feeding LUCIs; and (4) LINO-NIRVANA - an NGS/MCAO imager and interferometer system. AO performance of the current systems is presented along with proposed performances for the newer systems taking into account the future instrumentation.
    ISSN
    0277-786X
    DOI
    10.1117/12.2231783
    Version
    Final published version
    Additional Links
    http://proceedings.spiedigitallibrary.org/proceeding.aspx?doi=10.1117/12.2231783
    ae974a485f413a2113503eed53cd6c53
    10.1117/12.2231783
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