@inproceedings{oai:jaxa.repo.nii.ac.jp:00003053,
 author = {Mede, Kyle and Brandt, Timothy D. and 成田, 憲保 and 高橋, 安大 and Mede, Kyle and Brandt, Timothy D. and Narita, Norio and Takahashi, Yasuhiro H.},
 book = {宇宙航空研究開発機構特別資料, JAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe},
 month = {Mar},
 note = {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, 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., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730027076, レポート番号: JAXA-SP-17-010E},
 pages = {353--355},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {Markov Chain Monte Carlo Simulations and Binary Orbital Elements},
 volume = {JAXA-SP-17-010E},
 year = {2018}
}