Production of 8.4 m primary mirror segments for GMT
dc.contributor.author | Martin, H.M. | |
dc.contributor.author | Ceragioli, R. | |
dc.contributor.author | Gasho, V. | |
dc.contributor.author | Jannuzi, B.T. | |
dc.contributor.author | Kim, D.W. | |
dc.contributor.author | Kingsley, J.S. | |
dc.contributor.author | Law, K. | |
dc.contributor.author | Loeff, A. | |
dc.contributor.author | Lutz, R.D. | |
dc.contributor.author | Meyen, S. | |
dc.contributor.author | Oh, C.J. | |
dc.contributor.author | Tuell, M.T. | |
dc.contributor.author | Weinberger, S.N. | |
dc.contributor.author | West, S.C. | |
dc.contributor.author | Whitsitt, R. | |
dc.contributor.author | Wortley, R. | |
dc.date.accessioned | 2022-12-15T22:40:56Z | |
dc.date.available | 2022-12-15T22:40:56Z | |
dc.date.issued | 2022 | |
dc.identifier.citation | Martin, H. M., Ceragioli, R., Gasho, V., Jannuzi, B. T., Kim, D. W., Kingsley, J. S., Law, K., Loeff, A., Lutz, R. D., Meyen, S., Oh, C. J., Tuell, M. T., Weinberger, S. N., West, S. C., Whitsitt, R., & Wortley, R. (2022). Production of 8.4 m primary mirror segments for GMT. Proceedings of SPIE - The International Society for Optical Engineering, 12188. | |
dc.identifier.isbn | 9781510653573 | |
dc.identifier.issn | 0277-786X | |
dc.identifier.doi | 10.1117/12.2630378 | |
dc.identifier.uri | http://hdl.handle.net/10150/667187 | |
dc.description.abstract | The Richard F. Caris Mirror Lab at the University of Arizona continues production of 8.4 m lightweight honeycomb segments for the primary mirror of the Giant Magellan Telescope. GMT's 25 m primary mirror consists of a center segment surrounded by six off-axis segments, with an additional off-axis segment to allow continuous operation as segments are removed for coating. We cast the sixth segment (5 off-axis segments + center segment) in March 2021. As of June 2022 we have tentatively completed polishing of the third off-axis segment, and we are in the process of grinding the optical surface of off-axis Segment 5. For Segment 3, we improved the measurement accuracy for small-scale structure near the edge of the mirror, which has been a challenge for the off-axis segments. In addition to full-aperture interferometry and deflectometry, we used a 20 cm test plate to obtain high-resolution interferometric measurements of the edge. © COPYRIGHT SPIE. Downloading of the abstract is permitted for personal use only. | |
dc.language.iso | en | |
dc.publisher | SPIE | |
dc.rights | Copyright © 2022 SPIE. | |
dc.rights.uri | http://rightsstatements.org/vocab/InC/1.0/ | |
dc.subject | aspheres | |
dc.subject | Giant Magellan Telescope | |
dc.subject | off-axis | |
dc.subject | optical fabrication | |
dc.subject | optical testing | |
dc.subject | telescopes | |
dc.title | Production of 8.4 m primary mirror segments for GMT | |
dc.type | Proceedings | |
dc.type | text | |
dc.contributor.department | Steward Observatory, University of Arizona | |
dc.contributor.department | College of Optical Sciences, University of Arizona | |
dc.identifier.journal | Proceedings of SPIE - The International Society for Optical Engineering | |
dc.description.note | Immediate access | |
dc.description.collectioninformation | 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. | |
dc.eprint.version | Final published version | |
dc.source.journaltitle | Proceedings of SPIE - The International Society for Optical Engineering | |
refterms.dateFOA | 2022-12-15T22:40:56Z |