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    Status of mirror segment production for the Giant Magellan Telescope

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    Author
    Martin, H. M.
    Burge, J. H.
    Davis, J. M.
    Kim, D. W.
    Kingsley, J. S.
    Law, K.
    Loeff, A.
    Lutz, R. D.
    Merrill, C.
    Strittmatter, P. A.
    Tuell, M. T.
    Weinberger, S. N.
    West, S. C.
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    Affiliation
    Univ Arizona, Steward Observ
    Univ Arizona, Ctr Opt Sci
    Issue Date
    2016-07-22
    Keywords
    Giant Magellan Telescope
    telescopes
    optical fabrication
    optical testing
    off-axis
    aspheres
    
    Metadata
    Show full item record
    Publisher
    SPIE-INT SOC OPTICAL ENGINEERING
    Citation
    H. M. Martin ; J. H. Burge ; J. M. Davis ; D. W. Kim ; J. S. Kingsley ; K. Law ; A. Loeff ; R. D. Lutz ; C. Merrill ; P. A. Strittmatter ; M. T. Tuell ; S. N. Weinberger and S. C. West " Status of mirror segment production for the Giant Magellan Telescope ", Proc. SPIE 9912, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation II, 99120V (July 22, 2016); doi:10.1117/12.2234491; http://dx.doi.org/10.1117/12.2234491
    Journal
    ADVANCES IN OPTICAL AND MECHANICAL TECHNOLOGIES FOR TELESCOPES AND INSTRUMENTATION II
    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 Richard F. Caris Mirror Lab at the University of Arizona is responsible for production of the eight 8.4 m segments for the primary mirror of the Giant Magellan Telescope, including one spare off-axis segment. We report on the successful casting of Segment 4, the center segment. Prior to generating the optical surface of Segment 2, we carried out a major upgrade of our 8.4 m Large Optical Generator. The upgrade includes new hardware and software to improve accuracy, safety, reliability and ease of use. We are currently carrying out an upgrade of our 8.4 m polishing machine that includes improved orbital polishing capabilities. We added and modified several components of the optical tests during the manufacture of Segment 1, and we have continued to improve the systems in preparation for Segments 2-8. We completed two projects that were prior commitments before GMT Segment 2: casting and polishing the combined primary and tertiary mirrors for the LSST, and casting and generating a 6.5 m mirror for the Tokyo Atacama Observatory.
    Note
    SPIE grants to authors of papers published in an SPIE Journal or Proceedings the right to post an author-prepared version or an official version (preferred version) of the published paper on an internal or external server controlled exclusively by the author/employer, provided that (a) such posting is noncommercial in nature and the paper is made available to users without charge; (b) an appropriate copyright notice and full citation appear with the paper, and (c) a link to SPIE's official online version of the abstract is provided using the DOI (Document Object Identifier) link.
    ISSN
    0277-786X
    DOI
    10.1117/12.2234491
    Version
    Final published version
    Additional Links
    http://proceedings.spiedigitallibrary.org/proceeding.aspx?doi=10.1117/12.2234491
    ae974a485f413a2113503eed53cd6c53
    10.1117/12.2234491
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