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    Nancy Grace Roman Space Telescope Coronagraph Instrument Overview and Status

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    Author
    Bailey, V.P.
    Bendek, E.
    Monacelli, B.
    Baker, C.
    Bedrosian, G.
    Cady, E.
    Douglas, E.S.
    Groff, T.
    Hildebrandt, S.R.
    Kasdin, N.J.
    Krist, J.
    Macintosh, B.
    Mennesson, B.
    Morrissey, P.
    Poberezhskiy, I.
    Subedi, H.B.
    Rhodes, J.
    Roberge, A. cc
    Ygouf, M.
    Zellem, R.T.
    Zhao, F.
    Zimmerman, N.T.
    Show allShow less
    Affiliation
    Steward Observatory, The Department of Astronomy, The University of Arizona
    Issue Date
    2023-10-05
    Keywords
    circumstellar disks
    coronagraphy
    deformable mirrors
    electron multiplying CCDs
    exoplanets
    high-contrast imaging
    Roman Space Telescope
    
    Metadata
    Show full item record
    Publisher
    SPIE
    Citation
    Vanessa P. Bailey, Eduardo Bendek, Brian Monacelli, Caleb Baker, Gasia Bedrosian, Eric Cady, Ewan S. Douglas, Tyler Groff, Sergi R. Hildebrandt, N. Jeremy Kasdin, John Krist, Bruce Macintosh, Bertrand Mennesson, Patrick Morrissey, Ilya Poberezhskiy, Hari B. Subedi, Jason Rhodes, Aki Roberge, Marie Ygouf, Robert T. Zellem, Feng Zhao, Neil T. Zimmerman, "Nancy Grace Roman Space Telescope coronagraph instrument overview and status," Proc. SPIE 12680, Techniques and Instrumentation for Detection of Exoplanets XI, 126800T (5 October 2023); https://doi.org/10.1117/12.2679036
    Journal
    Proceedings of SPIE - The International Society for Optical Engineering
    Rights
    © 2023 SPIE. (2023) Published by 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 Nancy Grace Roman Space Telescope Coronagraph Instrument is a critical technology demonstrator for NASA’s Habitable Worlds Observatory. With a predicted visible-light flux ratio detection limit of 10−8 or better, it will be capable of reaching new areas of parameter space for both gas giant exoplanets and circumstellar disks. It is in the final stages of integration and test at the Jet Propulsion Laboratory, with an anticipated delivery to payload integration in the coming year. This paper will review the instrument systems, observing modes, potential observing applications, and overall progress toward instrument integration and test. © 2023 SPIE.
    Note
    Immediate access
    ISSN
    0277-786X
    ISBN
    978-151066574-3
    DOI
    10.1117/12.2679036
    Version
    Final Published Version
    ae974a485f413a2113503eed53cd6c53
    10.1117/12.2679036
    Scopus Count
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    UA Faculty Publications

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