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    Keck Planet Imager and Characterizer: concept and phased implementation

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    Author
    Mawet, D.
    Wizinowich, P.
    Dekany, R.
    Chun, M.
    Hall, D.
    Cetre, S.
    Guyon, O.
    Wallace, J. K.
    Bowler, B.
    Liu, M.
    Ruane, G.
    Serabyn, E.
    Bartos, R.
    Wang, J.
    Vasisht, G.
    Fitzgerald, M.
    Skemer, A.
    Ireland, M.
    Fucik, J.
    Fortney, J.
    Crossfield, I.
    Hu, R.
    Benneke, B.
    Show allShow less
    Affiliation
    Univ Arizona, Lunar & Planetary Lab
    Issue Date
    2016-07-26
    Keywords
    Exoplanets
    high contrast imaging
    high contrast high resolution spectroscopy
    small inner working angle coronagraphy
    vortex coronagraph
    on-axis segmented telescopes
    apodization
    Extremely Large Telescopes
    
    Metadata
    Show full item record
    Publisher
    SPIE-INT SOC OPTICAL ENGINEERING
    Citation
    D. Mawet ; P. Wizinowich ; R. Dekany ; M. Chun ; D. Hall ; S. Cetre ; O. Guyon ; J. K. Wallace ; B. Bowler ; M. Liu ; G. Ruane ; E. Serabyn ; R. Bartos ; J. Wang ; G. Vasisht ; M. Fitzgerald ; A. Skemer ; M. Ireland ; J. Fucik ; J. Fortney ; I. Crossfield ; R. Hu and B. Benneke " Keck Planet Imager and Characterizer: concept and phased implementation ", Proc. SPIE 9909, Adaptive Optics Systems V, 99090D (July 26, 2016); doi:10.1117/12.2233658; http://dx.doi.org/10.1117/12.2233658
    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 Keck Planet Imager and Characterizer (KPIC) is a cost-effective upgrade path to the W.M. Keck observatory (WMKO) adaptive optics (AO) system, building on the lessons learned from first and second-generation extreme AO (ExA0) coronagraphs. KPIC will explore new scientific niches in exoplanet science, while maturing critical technologies and systems for future ground-based (TMT, FELT, GMT) and space-based planet imagers (HabEx, LUVOIR). The advent of fast low-noise IR cameras (IR-APD, MKIDS, electron injectors), the rapid maturing of efficient wavefront sensing (WFS) techniques (Pyramid, Zernike), small inner working angle (IWA) coronagraphs (e.g., vortex) and associated low-order wavefront sensors (LOWFS), as well as recent breakthroughs in high contrast high resolution spectroscopy, open new direct exoplanet exploration avenues that are complementary to planet imagers such as VLT-SPHERE and the Gemini Planet Imager (GPI). For instance, the search and detailed characterization of planetary systems on solar-system scales around late-type stars, mostly beyond SPHERE and GPI's reaches, can be initiated now at WMKO.
    ISSN
    0277-786X
    DOI
    10.1117/12.2233658
    Version
    Final published version
    Additional Links
    http://proceedings.spiedigitallibrary.org/proceeding.aspx?doi=10.1117/12.2233658
    ae974a485f413a2113503eed53cd6c53
    10.1117/12.2233658
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