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    Combination of apodized pupil and phase mask coronagraph for SCExAO at Subaru Telescope

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    Author
    Nishikawa, J.
    Murakami, N.
    Lozi, J.
    Guyon, O. cc
    Habu, K.
    Ichien, H.
    Yoneta, K.
    Sudo, S.
    Kumaki, K.
    Kumagaih, S.
    Jovanovic, N.
    Martinache, F.
    Show allShow less
    Affiliation
    Steward Observatory, University of Arizona
    College of Optical Sciences, University of Arizona
    Issue Date
    2020
    Keywords
    Adaptive optics
    Apodizer
    Coronagraph
    Exoplanet
    Phase mask
    Shaped pupil
    
    Metadata
    Show full item record
    Publisher
    SPIE
    Citation
    Nishikawa, J., Murakami, N., Lozi, J., Guyon, O., Habu, K., Ichien, H., Yoneta, K., Sudo, S., Kumaki, K., Kumagaih, S., Jovanovic, N., & Martinache, F. (2020). Combination of apodized pupil and phase mask coronagraph for SCExAO at Subaru Telescope. Proceedings of SPIE - The International Society for Optical Engineering, 11447.
    Journal
    Proceedings of SPIE - The International Society for Optical Engineering
    Rights
    Copyright © 2021 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
    Subaru telescope has been operating a high-contrast imaging instruments called Subaru coronagraphic extreme adaptive optics (SCExAO) which is used for exoplanet research. We are developing phase mask coronagraphs using photonic crystal wave plates inside the SCExAO. An eight-octant phase mask (8OPM) of three-layer achromatic structure has been fabricated as a second generation. It was designed for J and H band to reach 10-5 contrast, and Ks band to 10-4. A retardation and a coronagraphic performance of the 8OPM were confirmed almost as designed at 1550nm. An apodised (binary shaped) pupil to be used with the 8OPM was also studied to suppress diffracted light by the secondary shadow and spiders. We confirmed a performance of the combination of the apodizer and the 8OPM at visible wavelengths in a lab. We optimized the apodizer for a pupil of the SCExAO where we obtained a transmission of 50 % and a contrast of 10-4 at the center and 10-6 at outer region. We manufactured the designed apodizer to be installed in SCExAO for infrared observations. © 2020 SPIE
    Note
    Immediate access
    ISSN
    0277-786X
    ISBN
    9781510636811
    DOI
    10.1117/12.2560839
    Version
    Final published version
    ae974a485f413a2113503eed53cd6c53
    10.1117/12.2560839
    Scopus Count
    Collections
    UA Faculty Publications

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