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    FIRST, a pupil-remapping fiber interferometer at the Subaru Telescope: On-sky results

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    Author
    Vievard, S.
    Huby, E.
    Lacour, S.
    Barjot, K.
    Martin, G.
    Cvetojevic, N.
    Deo, V.
    Guyon, O. cc
    Lozi, J.
    Kotani, T.
    Jovanovic, N.
    Marchis, F.
    Duchêne, G.
    Lapeyrere, V.
    Rouan, D.
    Perrin, G.
    Show allShow less
    Affiliation
    College of Optical Sciences, University of Arizona
    Issue Date
    2020
    Keywords
    High angular resolution
    High contrast imaging
    Interferometry
    Pupil remapping
    Single-mode fibers
    
    Metadata
    Show full item record
    Publisher
    SPIE
    Citation
    Vievard, S., Huby, E., Lacour, S., Barjot, K., Martin, G., Cvetojevic, N., ... & Perrin, G. (2020, December). FIRST, a pupil-remapping fiber interferometer at the Subaru Telescope: on-sky results. In Optical and Infrared Interferometry and Imaging VII (Vol. 11446, p. 1144629). International Society for Optics and Photonics.
    Journal
    Proceedings of SPIE - The International Society for Optical Engineering
    Rights
    Copyright © 2020 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
    FIRST, the Fibered Imager foR a Single Telescope, is a spectro-imager using single-mode fibers for pupil remap- ping, allowing measurements beyond the telescope diffraction limit. Integrated on the Subaru Coronagraphic Extreme Adaptive Optics instrument at the Subaru Telescope, it benefits from a very stable visible light wave- front allowing to acquire long exposure and operate on significantly fainter sources than previously possible. On-sky results demonstrated the ability of the instrument to detect stellar companions separated 43mas in the case of the Capella binary system. A similar approach on an extremely large telescope would offer unique scientific opportunities for companion detection and characterization at very high angular resolution. © COPYRIGHT SPIE. Downloading of the abstract is permitted for personal use only.
    Note
    Immediate access
    ISSN
    0277-786X
    ISBN
    9781510000000
    DOI
    10.1117/12.2563033
    Version
    Final published version
    ae974a485f413a2113503eed53cd6c53
    10.1117/12.2563033
    Scopus Count
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    UA Faculty Publications

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