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The Seimei telescope project and technical developments.

Authors :
Kurita, Mikio
Kino, Masaru
Iwamuro, Fumihide
Ohta, Kouji
Nogami, Daisaku
Izumiura, Hideyuki
Yoshida, Michitoshi
Matsubayashi, Kazuya
Kuroda, Daisuke
Nakatani, Yoshikazu
Yamamoto, Kodai
Tsutsui, Hironori
Iribe, Masatsugu
Jikuya, Ichiro
Ohtani, Hiroshi
Shibata, Kazunari
Takahashi, Keisuke
Tokoro, Hitoshi
Maihara, Toshinori
Nagata, Tetsuya
Source :
Publications of the Astronomical Society of Japan. Jun2020, Vol. 72 Issue 3, p1-11. 11p.
Publication Year :
2020

Abstract

An overview of the Seimei telescope, a 3.8 m optical infrared telescope located on Mt. Chikurinji in the Okayama prefecture of Japan, is presented. Seimei is a segmented-mirror telescope whose primary mirror consists of 18 petal-shaped segments. The telescope tube supporting the thin segmented mirrors is structurally incorporated within large arc-rails providing the elevation axis. The tube has a light-weight homologous structure designed with a genetic algorithm. The total weight of the telescope tube, including 1.4-ton optics, is only 8 tons. By virtue of its light weight, the telescope is able to point at an object anywhere in the observable sky within one minute. The telescope is operated by Kyoto University in collaboration with the National Astronomical Observatory of Japan (NAOJ). Half of the telescope time is used by Kyoto University. The remaining time is open to the Japanese astronomical community. NAOJ is responsible for the management of the open-use time, including handling of the observation proposals. The telescope is now regularly performing scientific observations on the basis of a variety of proposals. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
00046264
Volume :
72
Issue :
3
Database :
Academic Search Index
Journal :
Publications of the Astronomical Society of Japan
Publication Type :
Academic Journal
Accession number :
143880624
Full Text :
https://doi.org/10.1093/pasj/psaa036