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Markov Chain Monte Carlo Simulations and Binary Orbital Elements
https://jaxa.repo.nii.ac.jp/records/3053
https://jaxa.repo.nii.ac.jp/records/305376a4c718-0f16-41e2-a8c4-37fe9e77dccb
名前 / ファイル | ライセンス | アクション |
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AA1730027076.pdf (3.4 MB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2018-05-07 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Markov Chain Monte Carlo Simulations and Binary Orbital Elements | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_5794 | |||||
資源タイプ | conference paper | |||||
著者 |
Mede, Kyle
× Mede, Kyle× Brandt, Timothy D.× 成田, 憲保× 高橋, 安大× Mede, Kyle× Brandt, Timothy D.× Narita, Norio× Takahashi, Yasuhiro H. |
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著者所属 | ||||||
東京大学 | ||||||
著者所属 | ||||||
Princeton University | ||||||
著者所属 | ||||||
国立天文台 : 総合研究大学院大学(SOKENDAI) | ||||||
著者所属 | ||||||
東京大学 : 国立天文台 | ||||||
著者所属(英) | ||||||
en | ||||||
The University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Princeton University | ||||||
著者所属(英) | ||||||
en | ||||||
National Astronomical Observatory of Japan : The Graduate University for Advanced Studies (SOKENDAI) | ||||||
著者所属(英) | ||||||
en | ||||||
The University of Tokyo : National Astronomical Observatory of Japan | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構(JAXA) | |||||
出版者(英) | ||||||
出版者 | Japan Aerospace Exploration Agency (JAXA) | |||||
書誌情報 |
宇宙航空研究開発機構特別資料 en : JAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe 巻 JAXA-SP-17-010E, p. 353-355, 発行日 2018-03-09 |
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会議概要(会議名, 開催地, 会期, 主催者等)(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe (June 18-21, 2013. Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Recent simulations and observational data have been used to investigate the possibility of planet-planet scattering or Kozai oscillations to explain the formation of certain non-solar-like planetary systems. Markov Chain Monte Carlo (MCMC) simulations have benefits compared to standard Monte Carlo ones. With these advantages in mind, an advanced three dimensional MCMC simulator has been written to investigate the orbital solutions to the τ Boo system in order to better understand its possible formation history. | |||||
内容記述 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 形態: カラー図版あり | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Physical characteristics: Original contains color illustrations | |||||
ISSNONLINE | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 2433-2232 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA1730027076 | |||||
レポート番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | レポート番号: JAXA-SP-17-010E |