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    The University of Tokyo Atacama Observatory 6.5m Telescope: Design of mirror coating system and its performances II

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    Author
    Takahashi, H.
    Yoshii, Y.
    Doi, M.
    Miyata, T.
    Kohno, K.
    Tanaka, M.
    Motohara, K.
    Minezaki, T.
    Sako, S.
    Morokuma, T.
    Tanabé, T.
    Hatsukade, B.
    Konishi, M.
    Kamizuka, T.
    Asano, K.
    Sameshima, H.
    Kato, N.
    Numata, M.
    Aoki, T.
    Soyano, T.
    Tarusawa, K.
    Kawai, Y.
    Ogawa, H.
    Show allShow less
    Affiliation
    Steward Observatory, University of Arizona
    Issue Date
    2020
    Keywords
    Atacama
    Co. Chajnantor
    Coating
    Evaporation
    Mirror
    TAO
    
    Metadata
    Show full item record
    Publisher
    SPIE
    Citation
    Takahashi, H., Yoshii, Y., Doi, M., Miyata, T., Kohno, K., Tanaka, M., ... & Ogawa, H. (2020, December). The University of Tokyo Atacama Observatory 6.5 m Telescope: Design of mirror coating system and its performances II. In Ground-based and Airborne Telescopes VIII (Vol. 11445, p. 1144564). 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
    The telescope of the University of Tokyo Atacama Observatory has a primary mirror with a diameter in 6.5m. In order to fabricate the reflecting film initially on the mirror surface and to maintain its optical performance over a long period, a mirror{coating facility will be installed in operation building beside enclosure of the telescope at the summit of Co. Chajnantor (5,640m). The facility consists of mirror coating chamber, cleaning unit for stripping off the old film and clean-up the mirror, and a cart with a lifter for handling the primary mirror cell. Almost all equipment, including the main chamber, was completed by early 2020 and engaged as a mirror coating facility. In order to optimize the coating parameters, comprehensive performance tests were carried out (without primary mirror cell which plays a role of a part of chamber). The evaluation items are how long it takes to reach the target vacuum level and parameters of the current, voltage, and application time during ion bombardment and aluminization. Through iterating test, we were able to obtain each parameter that ultimately met the requirements of the TAO telescope mirror. © COPYRIGHT SPIE. Downloading of the abstract is permitted for personal use only.
    Note
    Immediate access
    ISSN
    0277-786X
    ISBN
    9781510000000
    DOI
    10.1117/12.2561871
    Version
    Final published version
    ae974a485f413a2113503eed53cd6c53
    10.1117/12.2561871
    Scopus Count
    Collections
    UA Faculty Publications

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