文献

J-GLOBAL ID：202002279170403467   整理番号：20A2223842

OGLE-2017-BLG-0406:Spitzerマイクロレンズ視差は内部銀河円盤における土星-質量惑星軌道M-dwarfホストを明らかにする【JST・京大機械翻訳】

OGLE-2017-BLG-0406: Spitzer Microlens Parallax Reveals Saturn-mass Planet Orbiting M-dwarf Host in the Inner Galactic Disk

著者 (120件)： Hirao Yuki (Department of Earth and Space Science, Graduate School of Science, Osaka University, 1-1 Machikaneyama, Toyonaka, Osaka 560-0043, Japan) ,  Hirao Yuki (Laboratory for Exoplanets and Stellar Astrophysics, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA) ,  Hirao Yuki (Department of Astronomy, University of Maryland, College Park, MD 20742, USA) ,  Bennett David P. (Laboratory for Exoplanets and Stellar Astrophysics, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA) ,  Bennett David P. (Department of Astronomy, University of Maryland, College Park, MD 20742, USA) ,  Ryu Yoon-Hyun (Korea Astronomy and Space Science Institute, Daejon 34055, Republic of Korea) ,  Koshimoto Naoki (Department of Astronomy, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan) ,  Udalski Andrzej (Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, 00-478 Warszawa, Poland) ,  Yee Jennifer C. (Center for Astrophysics | Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA) ,  Sumi Takahiro (Department of Earth and Space Science, Graduate School of Science, Osaka University, 1-1 Machikaneyama, Toyonaka, Osaka 560-0043, Japan) ,  Bond Ian A. (Institute of Information and Mathematical Sciences, Massey University, Private Bag 102-904, North Shore Mail Centre, Auckland, New Zealand) ,  Shvartzvald Yossi (Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot 76100, Israel) ,  Abe Fumio (Institute for Space-Earth Environmental Research, Nagoya University, Nagoya 464-8601, Japan) ,  Barry Richard K. (Astrophysics Science Division, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA) ,  Bhattacharya Aparna (Laboratory for Exoplanets and Stellar Astrophysics, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA) ,  Bhattacharya Aparna (Department of Astronomy, University of Maryland, College Park, MD 20742, USA) ,  Donachie Martin (Department of Physics, University of Auckland, Private Bag 92019, Auckland, New Zealand) ,  Fukui Akihiko (Department of Earth and Planetary Science, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan) ,  Fukui Akihiko (Instituto de Astrofisica de Canarias, Via Lactea s/n, E-38205 La Laguna, Tenerife, Spain) ,  Itow Yoshitaka (Institute for Space-Earth Environmental Research, Nagoya University, Nagoya 464-8601, Japan) ,  Kondo Iona (Department of Earth and Space Science, Graduate School of Science, Osaka University, 1-1 Machikaneyama, Toyonaka, Osaka 560-0043, Japan) ,  Alex Li Man Cheung (Department of Physics, University of Auckland, Private Bag 92019, Auckland, New Zealand) ,  Matsubara Yutaka (Institute for Space-Earth Environmental Research, Nagoya University, Nagoya 464-8601, Japan) ,  Matsuo Taro (Department of Earth and Space Science, Graduate School of Science, Osaka University, 1-1 Machikaneyama, Toyonaka, Osaka 560-0043, Japan) ,  Miyazaki Shota (Department of Earth and Space Science, Graduate School of Science, Osaka University, 1-1 Machikaneyama, Toyonaka, Osaka 560-0043, Japan) ,  Muraki Yasushi (Institute for Space-Earth Environmental Research, Nagoya University, Nagoya 464-8601, Japan) ,  Nagakane Masayuki (Department of Earth and Space Science, Graduate School of Science, Osaka University, 1-1 Machikaneyama, Toyonaka, Osaka 560-0043, Japan) ,  Ranc Clement (Laboratory for Exoplanets and Stellar Astrophysics, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA) ,  Rattenbury Nicholas J. (Department of Physics, University of Auckland, Private Bag 92019, Auckland, New Zealand) ,  Suematsu Haruno (Department of Earth and Space Science, Graduate School of Science, Osaka University, 1-1 Machikaneyama, Toyonaka, Osaka 560-0043, Japan) ,  Shibai Hiroshi (Department of Earth and Space Science, Graduate School of Science, Osaka University, 1-1 Machikaneyama, Toyonaka, Osaka 560-0043, Japan) ,  Suzuki Daisuke (Department of Earth and Space Science, Graduate School of Science, Osaka University, 1-1 Machikaneyama, Toyonaka, Osaka 560-0043, Japan) ,  Tristram Paul J. (.University of Canterbury, Mount John Observatory, P.O. Box 56, Lake Tekapo 8770, New Zealand) ,  Yonehara Atsunori (Department of Physics, Faculty of Science, Kyoto Sangyo University, Kyoto 603-8555, Japan) ,  The MOA Collaboration ,  Skowron J. (Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, 00-478 Warszawa, Poland) ,  Poleski R. (Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, 00-478 Warszawa, Poland) ,  Poleski R. (Department of Astronomy, Ohio State University, 140 West 18th Avenue, Columbus, OH 43210, USA) ,  Mroz P. (Division of Physics, Mathematics, and Astronomy, California Institute of Technology, Pasadena, CA 91125, USA) ,  Szymanski M. K. (Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, 00-478 Warszawa, Poland) ,  Soszynski I. (Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, 00-478 Warszawa, Poland) ,  Kozlowski S. (Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, 00-478 Warszawa, Poland) ,  Pietrukowicz P. (Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, 00-478 Warszawa, Poland) ,  Ulaczyk K. (Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, 00-478 Warszawa, Poland) ,  Rybicki K. (Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, 00-478 Warszawa, Poland) ,  Iwanek P. (Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, 00-478 Warszawa, Poland) ,  The OGLE Collaboration ,  D. Albrow Michael (University of Canterbury, Department of Physics and Astronomy, Private Bag 4800, Christchurch 8020, New Zealand) ,  Chung Sun-Ju (Korea Astronomy and Space Science Institute, Daejon 34055, Republic of Korea) ,  Chung Sun-Ju (Korea University of Science and Technology, Daejeon 34113, Republic of Korea) ,  Gould Andrew (Korea Astronomy and Space Science Institute, Daejon 34055, Republic of Korea) ,  Gould Andrew (Max-Planck-Institute for Astronomy, Konigstuhl 17, D-69117 Heidelberg, Germany) ,  Gould Andrew (Department of Astronomy, Ohio State University, 140 W. 18th Avenue, Columbus, OH 43210, USA) ,  Han Cheongho (Department of Physics, Chungbuk National University, Cheongju 28644, Republic of Korea) ,  Hwang Kyu-Ha (Korea Astronomy and Space Science Institute, Daejon 34055, Republic of Korea) ,  Jung Youn Kil (Korea Astronomy and Space Science Institute, Daejon 34055, Republic of Korea) ,  Shin In-Gu (Korea Astronomy and Space Science Institute, Daejon 34055, Republic of Korea) ,  Zang Weicheng (Physics Department and Tsinghua Centre for Astrophysics, Tsinghua University, Beijing 100084, People’s Republic of China) ,  Cha Sang-Mok (Korea Astronomy and Space Science Institute, Daejon 34055, Republic of Korea) ,  Cha Sang-Mok (School of Space Research, Kyung Hee University, Yongin, Kyeonggi 17104, Republic of Korea) ,  Kim Dong-Jin (Korea Astronomy and Space Science Institute, Daejon 34055, Republic of Korea) ,  Kim Hyoun-Woo (Korea Astronomy and Space Science Institute, Daejon 34055, Republic of Korea) ,  Kim Seung-Lee (Korea Astronomy and Space Science Institute, Daejon 34055, Republic of Korea) ,  Kim Seung-Lee (Korea University of Science and Technology, Daejeon 34113, Republic of Korea) ,  Lee Chung-Uk (Korea Astronomy and Space Science Institute, Daejon 34055, Republic of Korea) ,  Lee Dong-Joo (Korea Astronomy and Space Science Institute, Daejon 34055, Republic of Korea) ,  Lee Yongseok (Korea Astronomy and Space Science Institute, Daejon 34055, Republic of Korea) ,  Lee Yongseok (School of Space Research, Kyung Hee University, Yongin, Kyeonggi 17104, Republic of Korea) ,  Park Byeong-Gon (Korea Astronomy and Space Science Institute, Daejon 34055, Republic of Korea) ,  Park Byeong-Gon (Korea University of Science and Technology, Daejeon 34113, Republic of Korea) ,  Pogge Richard W. (Department of Astronomy, Ohio State University, 140 W. 18th Avenue, Columbus, OH 43210, USA) ,  The KMTNet Collaboration ,  Beichman Charles A. (IPAC, Mail Code 100-22, Caltech, 1200 E. California Boulevard, Pasadena, CA 91125, USA) ,  Bryden Geoffery (Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA) ,  Novati Sebastiano Calchi (IPAC, Mail Code 100-22, Caltech, 1200 E. California Boulevard, Pasadena, CA 91125, USA) ,  Carey Sean (IPAC, Mail Code 100-22, Caltech, 1200 E. California Boulevard, Pasadena, CA 91125, USA) ,  Gaudi B. Scott (Department of Astronomy, Ohio State University, 140 W. 18th Avenue, Columbus, OH 43210, USA) ,  Henderson Calen B. (IPAC, Mail Code 100-22, Caltech, 1200 E. California Boulevard, Pasadena, CA 91125, USA) ,  Zhu Wei (Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St. George Street, Toronto, ON M5S 3H8, Canada) ,  The Spitzer Team ,  Bachelet Etienne (Las Cumbres Observatory, 6740 Cortona Drive, Suite 102, Goleta, CA 93117, USA) ,  Bolt Greg (Craigie Observatory, Western Australia, Australia) ,  Christie Grant (Auckland Observatory, Auckland, New Zealand) ,  Hundertmark Markus (Astronomisches Rechen-Institut, Zentrum fuer Astronomie der Universitaet Heidelberg (ZAH), D-69120 Heidelberg, Germany) ,  Natusch Tim (Auckland Observatory, Auckland, New Zealand) ,  Natusch Tim (Institute for Radio Astronomy and Space Research (IRASR), AUT University, Auckland, New Zealand) ,  Maoz Dan (School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv 6997801, Israel) ,  McCormick Jennie (Farm Cove Observatory, Centre for Backyard Astrophysics, Pakuranga, Auckland, New Zealand) ,  A. Street Rachel (Las Cumbres Observatory, 6740 Cortona Drive, Suite 102, Goleta, CA 93117, USA) ,  Tan Thiam-Guan (Perth Exoplanet Survey Telescope, Perth, Australia) ,  Tsapras Yiannis (Astronomisches Rechen-Institut, Zentrum fuer Astronomie der Universitaet Heidelberg (ZAH), D-69120 Heidelberg, Germany) ,  The LCO and μFUN Follow-up Teams ,  Jorgensen U. G. (Niels Bohr Institute & Centre for Star and Planet Formation, University of Copenhagen Oster Voldgade 5, DK-1350-Copenhagen, Denmark) ,  Dominik M. (Centre for Exoplanet Science, SUPA School of Physics & Astronomy, University of St Andrews, North Haugh, St Andrews, KY16 9SS, UK) ,  Bozza V. (Dipartimento di Fisica “E.R. Caianiello,” Universita di Salerno, Via Giovanni Paolo II 132, I-84084, Fisciano, Italy) ,  Bozza V. (Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Napoli, Italy) ,  Skottfelt J. (Centre for Electronic Imaging, Department of Physical Sciences, The Open University, Milton Keynes, MK7 6AA, UK) ,  Snodgrass C. (Institute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh EH9 3HJ, UK) ,  Ciceri S. (Department of Astronomy, Stockholm University, AlbaNova University Centre, SE-106 91 Stockholm, Sweden) ,  Jaimes R. Figuera (Physics Department and Tsinghua Centre for Astrophysics, Tsinghua University, Beijing 100084, People’s Republic of China) ,  Jaimes R. Figuera (Centre for Exoplanet Science, SUPA School of Physics & Astronomy, University of St Andrews, North Haugh, St Andrews, KY16 9SS, UK) ,  Evans D. F. (Astrophysics Group, Keele University, Staffordshire, ST5 5BG, UK) ,  Peixinho N. (Centro de Astronomia (CITEVA), Universidad de Antofagasta, Avda. U. de Antofagasta 02800, Antofagasta, Chile) ,  Hinse T. C. (Chungnam National Universitys, Department of Astronomy and Space Science, 34134 Daejeon, Republic of Korea) ,  Burgdorf M. J. (Universitaet Hamburg, Faculty of Mathematics, Informatics and Natural Sciences, Department of Earth Sciences, Meteorological Institute, Bundesstrasse 55, D-20146 Hamburg, Germany) ,  Southworth J. (Astrophysics Group, Keele University, Staffordshire, ST5 5BG, UK) ,  Rahvar S. (Department of Physics, Sharif University of Technology, P.O. Box 11155-9161 Tehran, Iran) ,  Sajadian S. (Department of Physics, Isfahan University of Technology, Isfahan, Iran) ,  Rabus M. (Instituto de Astrofisica, Pontificia Universidad Catolica de Chile, Av. Vicuna Mackenna 4860, 7820436 Macul, Santiago, Chile) ,  Essen C. von (Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark) ,  Fujii Y. I. (Niels Bohr Institute & Centre for Star and Planet Formation, University of Copenhagen Oster Voldgade 5, DK-1350-Copenhagen, Denmark) ,  Fujii Y. I. (Institute for Advanced Research, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, 464-8601, Japan) ,  Campbell-White J. (Centre for Astrophysics & Planetary Science, The University of Kent, Canterbury CT2 7NH, UK) ,  Lowry S. (Centre for Astrophysics & Planetary Science, The University of Kent, Canterbury CT2 7NH, UK) ,  Helling C. (Centre for Exoplanet Science, SUPA School of Physics & Astronomy, University of St Andrews, North Haugh, St Andrews, KY16 9SS, UK) ,  Mancini L. (Dipartimento di Fisica, Universita di Roma Tor Vergata, Via della Ricerca Scientifica 1, I-00133 Roma, Italy) ,  Mancini L. (Max Planck Institute for Astronomy, Konigstuhl 17, D-69117 Heidelberg, Germany) ,  Mancini L. (INAF-Astrophysical Observatory of Turin, Via Osservatorio 20, I-10025 Pino Torinese, Italy) ,  Mancini L. (International Institute for Advanced Scientific Studies (IIASS), Via G. Pellegrino 19, I-84019 Vietri sul Mare (SA), Italy) ,  Haikala L. (Universidad de Atacama, Copiapo, Chile)
資料名： Astronomical Journal  (Astronomical Journal)
巻： 160  号： 2  ページ： 74 (20pp)  発行年： 2020年 
JST資料番号： W1567A  ISSN： 1538-3881  資料種別： 逐次刊行物 (A)
記事区分： 原著論文  発行国： イギリス (GBR)  言語： 英語 (EN)

抄録/ポイント： 太陽軌道における地上とSpitzer衛星の両方から観測された惑星マイクロレンズ現象OGLE-2017-BLG-0406の発見と解析を報告した。高倍率において,光曲線における異常は地上ベースの調査と追跡グループによって高密度に観察され,それは光曲線モデリングから惑星/ホスト質量比を有する惑星レンズによって説明されることが分かった。地上のみとSpitzer-”単独”データは,それぞれ2Dマイクロレンズパララックスベクトルに対して非常に強い一次元(1D)制約を提供する。組み合わせると,これらの収率は,ホストと惑星M_plant=0.41±0.05M_Jupの質量と質量の正確な測定をもたらした。このシステムは,D_L=5.2±0.5kpcの距離D_L=5.2±0.5kpcであり,そのホストは,レンズの運動学に従って,ディスク集団星である可能性が高い。ホストからの惑星の投影分離は(即ち,雪線の2倍以上)である。銀河ディスク運動学は,OGLE-IVデータに基づくソースの適切な運動の正確な測定から部分的に確立された。対照的に,ソースのGaia固有運動測定は,壊滅的10σ誤差に悩まされる。Please refer to the publisher for the copyright holders. Translated from English into Japanese by JST.【JST・京大機械翻訳】

シソーラス用語： 円板 ,  太陽 ,  *惑星 ,  *レンズ ,  土星 ,  *視差 ,  一次元 ,  *マイクロレンズ ,  銀河円盤 ,  高密度 ,  質量比

分類 (2件)： 惑星  (DB04020E) ,  恒星  (DB05000P)

タイトルに関連する用語 (7件)： マイクロレンズ ,  視差 ,  銀河円盤 ,  土星 ,  質量 ,  惑星 ,  軌道