Antarctic Telescope Project

(New) Dome Fuji Station, which is located at 3800m above sea level and whose temperature is quite low (-20℃～-80℃), is one of the best and unique sites for astronomical observations at infrared to submillimeter wavelengths on the ground. We are planning to constract two large terahertz and infrared t...

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Bibliographic Details
Main Authors: 中井 直正, 市川 隆, 瀬田 益道, 本山 秀明, 宮岡 宏, 他南極天文 コンソーシアム, Naomasa NAKAI, Takashi ICHIKAWA, Masumichi SETA, Hideaki MOTOYAMA, Hiroshi MIYAOKA, of Antarctica Astronomy Consortiaum
Format: Conference Object
Language:English
Published: 2016
Subjects:
Antarctic
Dome Fuji
Dome Fuji Station
Antarc*
国立極地研究所
Online Access:https://nipr.repo.nii.ac.jp/?action=repository_uri&item_id=11776
http://id.nii.ac.jp/1291/00011723/
https://nipr.repo.nii.ac.jp/?action=repository_action_common_download&item_id=11776&item_no=1&attribute_id=16&file_no=1
Description
Summary:(New) Dome Fuji Station, which is located at 3800m above sea level and whose temperature is quite low (-20℃～-80℃), is one of the best and unique sites for astronomical observations at infrared to submillimeter wavelengths on the ground. We are planning to constract two large terahertz and infrared telescopes at the station under the 9th JARE six-year plan, aiming at making astronomical observations including to search missing galaxies. 第4回極域科学シンポジウム特別セッション：[S] 南極研究の将来展望―第Ⅸ期6か年計画策定に向けて11月14日（木） 国立極地研究所 ２階大会議室

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