Status of mirror segment production for the Giant Magellan Telescope
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.
Affiliation
Univ Arizona, Steward ObservUniv Arizona, Ctr Opt Sci
Issue Date
2016-07-22
Metadata
Show full item recordPublisher
SPIE-INT SOC OPTICAL ENGINEERINGCitation
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/10.1117/12.2234491Rights
© 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
0277-786XVersion
Final published versionae974a485f413a2113503eed53cd6c53
10.1117/12.2234491
