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The University of Tokyo Atacama Observatory 6.5m Telescope: Design of mirror coating system and its performances II
Author
Takahashi, H.Yoshii, Y.
Doi, M.
Miyata, T.
Kohno, K.
Tanaka, M.
Motohara, K.
Minezaki, T.
Sako, S.
Morokuma, T.
Tanabé, T.
Hatsukade, B.
Konishi, M.
Kamizuka, T.
Asano, K.
Sameshima, H.
Kato, N.
Numata, M.
Aoki, T.
Soyano, T.
Tarusawa, K.
Kawai, Y.
Ogawa, H.
Affiliation
Steward Observatory, University of ArizonaIssue Date
2020
Metadata
Show full item recordPublisher
SPIECitation
Takahashi, H., Yoshii, Y., Doi, M., Miyata, T., Kohno, K., Tanaka, M., ... & Ogawa, H. (2020, December). The University of Tokyo Atacama Observatory 6.5 m Telescope: Design of mirror coating system and its performances II. In Ground-based and Airborne Telescopes VIII (Vol. 11445, p. 1144564). International Society for Optics and Photonics.Rights
Copyright © 2020 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 telescope of the University of Tokyo Atacama Observatory has a primary mirror with a diameter in 6.5m. In order to fabricate the reflecting film initially on the mirror surface and to maintain its optical performance over a long period, a mirror{coating facility will be installed in operation building beside enclosure of the telescope at the summit of Co. Chajnantor (5,640m). The facility consists of mirror coating chamber, cleaning unit for stripping off the old film and clean-up the mirror, and a cart with a lifter for handling the primary mirror cell. Almost all equipment, including the main chamber, was completed by early 2020 and engaged as a mirror coating facility. In order to optimize the coating parameters, comprehensive performance tests were carried out (without primary mirror cell which plays a role of a part of chamber). The evaluation items are how long it takes to reach the target vacuum level and parameters of the current, voltage, and application time during ion bombardment and aluminization. Through iterating test, we were able to obtain each parameter that ultimately met the requirements of the TAO telescope mirror. © COPYRIGHT SPIE. Downloading of the abstract is permitted for personal use only.Note
Immediate accessISSN
0277-786XISBN
9781510000000Version
Final published versionae974a485f413a2113503eed53cd6c53
10.1117/12.2561871