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Abstract: Antarctica provides a unique environment for astronomical observation, with cold, dry and stable air above the high Antarctic plateau. These summits offers the best seeing conditions, the darkest skies and the most transparent atmosphere of ground-based observing sites. Dome A is the highest point (4093 m) of Antarctica, the long polar winter night gives an unparalleled opportunity to conduct continuous observation for about four months. As the PLATeau Observatory (PLATO) was delivered to Dome A in January 2008, Chinese Small Telescope Array (CSTAR), four 14.5 cm Schmidt telescopes, was successfully installed on Dome A. Then Antarctic Survey Telescopes (AST3), three Schmidt telescopes with 50 cm aperture, started to be deployed on Dome A since 2012, which are the largest optical telescopes working in Antarctica. A number of new variables and exoplanet candidates were found through the remote-controlled observations. What is more exhilarating is that the optical counterpart of GW170817 was successfully captured by the second telescope of AST3. For the next generation of Chinese Antarctic telescopes, a 2.5 m optical/near-infrared telescope, so-called the Kunlun Dark Universe Telescope (KDUST), and the Dome A Terahertz Explorer-5 (DATE5), a 5 m sub-millimeter telescope can be expected in the early 2020s.
Language: English
東京大学・天文学教育研究センターでは2003年4月から, 院生コロキウムに引き続き, 談話会を開いています. 第一線で活躍されている研究者の方々を講師にお招きし, 最先端の研究成果をお話しいただきます. 講師の方には, 大学院生の参加者のことも考慮し, レビュー的な側面も含めた上で, ご自身の研究紹介をお願いしています.
| 13:30-14:30 | 院生コロキウム | 講義室 |
| 15:30-16:30 | 談話会 | 講義室 |
| 16:30- | お茶の時間 | 講義室横のお茶部屋~講師の方を交えて~ |
please replace _at_ to @
| # | Date | Speaker | Title | Chair |
| 318 | 2017/12/21 (Thu) 15:30 - 16:30 | 大屋 瑶子 (東京大学物理学専攻) | TBA | KK |
| 319 | 2017/12/22 (Fri) 13:30 - 14:30 | Lei Hu (Purple Mountain Observatory) | Chinese Antarctic Observatory at Dome A | MY |
詳細はこちら: 平成29 (2017) 年度談話会
| # | Date | Speaker | Title | Chair |
| 301 | 2017/4/13 (Thu) 15:30 - 16:30 | Tao WANG (IoA/U.Tokyo (4月から)) | New insights into the formation of the most massive galaxies at high redshifts | KK |
| 302 | 2017/4/20 (Thu) 15:30 - 16:30 | Matthew W. Johns (U. Arizona) | The Magellan Experience - Building a 6.5 Meter Optical/Infrared Telescope | TT |
| 303 | 2017/4/27 (Thu) 15:30 - 16:30 | 滝脇知也 (国立天文台 理論部) | 重力崩壊型超新星の爆発機構 | MY |
| 304 | 2017/5/11 (Thu) 15:30 - 16:30 | 樫山和己 (東京大学 物理学専攻) | A FRB in a bottle | MY |
| 305 | 2017/5/25 (Thu) 15:30 - 16:30 | 西村優里 (天文学教育研究センター (4月から)) | 低重元素量の矮小銀河における分子雲の化学組成 | KK |
| 306 | 2017/6/1 (Thu) 15:30 - 16:30 | 片岡章雅 (国立天文台フェロー) | Millimeter-wave polarization as a tool of investigating the planet formation | KK |
| 307 | 2017/6/15 (Thu) 15:30 - 16:30 | 端山和大 (東京大学 宇宙線研) | 重力波望遠鏡の現状と、検出から物理へ | MT |
| 308 | 2017/6/22 (Thu) 15:30 - 16:30 | 福島登志夫 (国立天文台) | 宇宙人存在問題 Question on Alien Civilization Existence | TT |
| 309 | 2017/7/13 (Thu) 15:30 - 16:30 | Ryan M. Lau (Caltech/JPL) | High Energy, Cool Transients: Investigating Infrared-Luminous Outbursts with Spitzer | KK |
| 310 | 2017/7/20 (Thu) 15:30 - 16:30 | 木坂将大 (青山学院大学) | 多波長観測で探るパルサー磁気圏構造 | MY |
| 311 | 2017/7/27 (Thu) 15:30 - 16:30 | 馬場彩 (東京大学 物理学専攻) | 超新星残骸のX線観測に関する最近の話題 | MY |
| 312 | 2017/10/12 (Thu) 15:30 - 16:30 | Jonathan Freundlich (Racah Institute of Physics, The Hebrew University) | Molecular gas reservoirs during the winding-down of star formation | MY |
| 313 | 2017/10/26 (Thu) 15:30 - 16:30 | Juergen Stutzki (Universitaet zu Koeln) | Optical depth of the Carbon 158 um line emission: high spectral resolution observations with SOFIA/upGREAT | KK |
| 314 | 2017/11/16 (Thu) 15:30 - 16:30 | 藤澤幸太郎 (早稲田大学) | Rapidly rotating substellar objects | MY |
| 315 | 2017/11/30 (Thu) 15:30 - 16:30 | 鈴木大介 (宇宙研 宇宙航空プロジェクト研究員) | Gravitational Microlensing Surveys for Exoplanets 重力マイクロレンズ法を用いた系外惑星探査 | MY |
| 316 | 2017/12/06 (Wed) 15:30 - 16:30 | 坂野正明 (Wise Babel Ltd) | (理系の)英文コミュニケーション — 履歴書から対レフェリー交渉迄 | KK |
| 317 | 2017/12/07 (Thu) 15:30 - 16:30 | 小西美穂子 (NAOJ 特任研究員) | アパチャマスキングで迫る原始惑星系円盤の主星最近傍領域 | MY |
