Optical technology for future telescopes
dc.contributor.author | Kim, Dae Wook | |
dc.contributor.author | Esparza, Marcos | |
dc.contributor.author | Quach, Henry | |
dc.contributor.author | Rodriguez, Stephanie | |
dc.contributor.author | Kang, Hyukmo | |
dc.contributor.author | Feng, Yi-Ting | |
dc.contributor.author | Choi, Heejoo | |
dc.date.accessioned | 2021-03-19T19:19:35Z | |
dc.date.available | 2021-03-19T19:19:35Z | |
dc.date.issued | 2021-01-15 | |
dc.identifier.citation | Kim, D. W., Esparza, M., Quach, H., Rodriguez, S., Kang, H., Feng, Y. T., & Choi, H. (2021, January). Optical technology for future telescopes. In Fourth International Conference on Photonics and Optical Engineering (Vol. 11761, p. 1176103). International Society for Optics and Photonics. | en_US |
dc.identifier.issn | 0277-786X | |
dc.identifier.doi | 10.1117/12.2586867 | |
dc.identifier.uri | http://hdl.handle.net/10150/657167 | |
dc.description.abstract | Various ground-based and space-based future telescope technologies are currently being conceptualized, designed, prototyped and tested to perform next generation astronomical sciences. They include (1) the alignment of segmented multi-order diffractive elements for the Nautilus space observatory; (2) the inflatable terahertz OASIS space telescope primary mirror characterization metrology; (3) active alignment of the laser truss-based Large Binocular Telescope prime focus camera; (4) the modular cross-dispersion spectroscopy unit, MOBIUS, used at the prime focal plane of the Large Binocular Telescope; (5) pupil segmentation topological optimization for future high contrast imaging telescopes; and (6) the optical design of the long slit UV spectroscopy space telescope Hyperion. This suite of enabling optical technologies and concept designs will redefine how humans understand the genesis and future of our universe. | en_US |
dc.language.iso | en | en_US |
dc.publisher | SPIE | en_US |
dc.rights | © 2021 SPIE. | en_US |
dc.rights.uri | http://rightsstatements.org/vocab/InC/1.0/ | en_US |
dc.source | Fourth International Conference on Photonics and Optical Engineering | |
dc.subject | Hyperion | en_US |
dc.subject | Large Binocular Telescope | en_US |
dc.subject | MOBIUS | en_US |
dc.subject | Nautilus | en_US |
dc.subject | OASIS | en_US |
dc.subject | Optical Metrology | en_US |
dc.subject | Pupil Segmentation | en_US |
dc.subject | Telescope Alignment | en_US |
dc.title | Optical technology for future telescopes | en_US |
dc.type | Article | en_US |
dc.contributor.department | Wyant College of Optical Sciences, University of Arizona | en_US |
dc.contributor.department | Department of Astronomy, University of Arizona | en_US |
dc.contributor.department | Steward Observatory, University of Arizona | en_US |
dc.contributor.department | Large Binocular Telescope Observatory, University of Arizona | en_US |
dc.identifier.journal | Proceedings of SPIE - The International Society for Optical Engineering | en_US |
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. | en_US |
dc.eprint.version | Final published version | en_US |
refterms.dateFOA | 2021-03-19T19:19:45Z |