천문학회보 (The Bulletin of The Korean Astronomical Society)
- 제42권2호
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- Pages.56.4-57
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- 2017
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- 1226-2692(pISSN)
Critical Design Status of the G-CLEF Flexure Control Camera
-
Oh, Jae Sok
(Korea Astronomy and Space Science Institute (KASI))
;
- Park, Chan (Korea Astronomy and Space Science Institute (KASI)) ;
-
Kim, Kang-Min
(Korea Astronomy and Space Science Institute (KASI))
;
-
Chun, Moo-Young
(Korea Astronomy and Space Science Institute (KASI))
;
-
Yu, Young Sam
(Korea Astronomy and Space Science Institute (KASI))
;
-
Lee, Sungho
(Korea Astronomy and Space Science Institute (KASI))
;
- Kim, Jihun (Korea Astronomy and Space Science Institute (KASI)) ;
- Szentgyorgyi, Andrew (Harvard-Smithsonian Center for Astrophysics) ;
- Podgorski, William (Harvard-Smithsonian Center for Astrophysics) ;
- Evans, Ian (Harvard-Smithsonian Center for Astrophysics) ;
- Mueller, Mark (Harvard-Smithsonian Center for Astrophysics) ;
- Uomoto, Alan (Observatories of the Carnegie Institution) ;
- Crane, Jeffrey (Observatories of the Carnegie Institution) ;
- Hare, Tyson (Observatories of the Carnegie Institution)
- 발행 : 2017.10.10
초록
The GMT-Consortium Large Earth Finder (G-CLEF) is the very first light instrument of the Giant Magellan Telescope (GMT) to be commissioned in 2022. The instrument is a fiber feed, optical band echelle spectrograph that is capable of extremely precise radial velocity measurement. Korea Astronomy and Space Science Institute (KASI) has been involved in the development of the G-CLEF as one member of the international consortium consisted of five astronomical institutes including Smithsonian Astrophysical Observatory (SAO), Observatories of the Carnegie Institution of Washington (OCIW). It is scheduled to have KASI side Critical Design Review in December 2017. In this presentation we will report the recent progress on the critical design activities for the G-CLEF Flexure Control Camera (FCC).
키워드