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The University of Tokyo Atacama Observatory 6.5m Telescope: Overview and construction status
Author
Yoshii, Y.Doi, M.
Miyata, T.
Kohno, K.
Tanaka, M.
Minezaki, T.
Sako, S.
Morokuma, T.
Tanabe, T.
Hatsukade, B.
Konishi, M.
Kamizuka, T.
Asano, K.
Sameshima, H.
Kato, N.
Numata, M.
Takahashi, H.
Aoki, T.
Soyano, T.
Tarusawa, K.
Yoshikawa, K.
Motohara, K.
Tamura, Y.
Koshida, S.
Handa, T.
Bronfman, L.
Ruiz, M.
Hamuy, M.
Mendez, R.
Escala, A.
Affiliation
Steward Observatory, The University of ArizonaIssue Date
2020
Metadata
Show full item recordPublisher
SPIECitation
Yoshii, Y., Doi, M., Miyata, T., Kohno, K., Tanaka, M., Minezaki, T., ... & Escala, A. (2020, December). The university of tokyo atacama observatory 6.5 m telescope: Overview and construction status. In Ground-based and Airborne Telescopes VIII (Vol. 11445, p. 1144514). 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
Institute of Astronomy, Graduate School of Science, the University of Tokyo is promoting the University of Tokyo Atacama Observatory Project, which is to construct an infrared-optimized 6.5m telescope at the summit of Co. Chajnantor (5640m altitude) in northern Chile. The high altitude and dry climate (PWV-0.5mm) realize transparent atmosphere in the infrared wavelength. The project is now approaching the final phase of the construction. Production of major components are almost completed: Production and preassembly test of a telescope mount and dome enclosure have been completed in Japan, and they are being transported to Chile. Three mirrors, the 6.5m primary, 0.9m secondary, and 1.1m-0.75m tertiary mirrors and their support systems have been all completed and tested in the USA. An aluminizing chamber have been fabricated in China, and its tests have been carried out in Japan. Development of two facility instruments, SWIMS and MIMIZUKU, are also completed. They were transported to the Subaru telescope, successfully saw the first light in 2018, and are confirmed to have the performance as designed. On-site construction work at the summit is now underway. Expansion of a summit access road from the ALMA concession was completed in 2019. Installation of foundation will follow, and then erection of the dome enclosure and a control building. The construction works are delayed by COVID-19, and we expect to complete the dome enclosure by Q3 of 2021. The telescope will be installed inside the dome and see the engineering first light by early 2022. © COPYRIGHT SPIE. Downloading of the abstract is permitted for personal use only.Note
Immediate accessISSN
0277-786XISBN
9781510000000Version
Final published versionae974a485f413a2113503eed53cd6c53
10.1117/12.2560238