Cosmic Evolution through UV Surveys (CETUS): Point spread function analysis of three mirror anastigmat telescope
Affiliation
Wyant College of Optical Sciences, University of ArizonaLarge Binocular Telescope Observatory, University Of Arizona
Issue Date
2021
Metadata
Show full item recordPublisher
SPIECitation
Ashcraft, J. N., Choi, H., Heap, S. R., Woodruff, R. A., & Kim, D. (2021). Cosmic Evolution through UV Surveys (CETUS): Point spread function analysis of three mirror anastigmat telescope. Proceedings of SPIE - The International Society for Optical Engineering.Rights
Copyright © 2021 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
Cosmic Evolution through UV Surveys (CETUS) is a concept for a UV space telescope that was studied with funding from NASA. The CETUS Final Report is posted at arXiv: 1909.10437, but post-report studies are continuing. Here, we describe telescope design options for CETUS including a trade study between a traditional on-axis three-mirror anastigmat (TMA) and freeform off-axis TMA solution considering their alignment sensitivity and tolerances. Different secondary support structures are explored for the on-axis design to analyze the irradiance distribution of the point-spread function (PSF) due to the pupil obscuration and how it influences the simulated starfield at the telescope focal planes. With rigorous and judicious analysis in geometrical optical design and physical wave propagation modeling, we aim to enable the next generation of spaceborne optical observatory for UV astronomy. © 2021 SPIE.Note
Immediate accessISSN
0277-786XISBN
9781510644786Version
Final published versionae974a485f413a2113503eed53cd6c53
10.1117/12.2598879