Author
Sebag, J.Gressler, W.
Liang, M.
Neill, D.
Araujo-Hauck, C.
Andrew, J.
Angeli, G.
Cho, M.
Claver, C.
Daruich, F.
Gessner, C.
Hileman, E.
Krabbendam, V.
Muller, G.
Poczulp, G.
Repp, R.
Wiecha, O.
Xin, B.
Kenagy, K.
Martin, H. M.
Tuell, M. T.
West, S. C.
Affiliation
Univ Arizona, Steward ObservIssue Date
2016-08-08
Metadata
Show full item recordPublisher
SPIE-INT SOC OPTICAL ENGINEERINGCitation
J. Sebag ; W. Gressler ; M. Liang ; D. Neill ; C. Araujo-Hauck ; J. Andrew ; G. Angeli ; M. Cho ; C. Claver ; F. Daruich ; C. Gessner ; E. Hileman ; V. Krabbendam ; G. Muller ; G. Poczulp ; R. Repp ; O. Wiecha ; B. Xin ; K. Kenagy ; H. M. Martin ; M. T. Tuell and S. C. West " LSST primary/tertiary monolithic mirror ", Proc. SPIE 9906, Ground-based and Airborne Telescopes VI, 99063E (August 8, 2016); doi:10.1117/12.2230012; http://dx.doi.org/10.1117/12.2230012Rights
© 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
At the core of the Large Synoptic Survey Telescope (LSST) three-mirror optical design is the primary/tertiary (M1M3) mirror that combines these two large mirrors onto one monolithic substrate. The M1M3 mirror was spin cast and polished at the Steward Observatory Mirror Lab at The University of Arizona (formerly SOML, now the Richard F. Caris Mirror Lab at the University of Arizona (RFCML)). Final acceptance of the mirror occurred during the year 2015 and the mirror is now in storage while the mirror cell assembly is being fabricated. The M1M3 mirror will be tested at RFCML after integration with its mirror cell before being shipped to Chile.ISSN
0277-786XVersion
Final published versionae974a485f413a2113503eed53cd6c53
10.1117/12.2230012
