凌日時間變分法 (Chinese Wikipedia)

Analysis of information sources in references of the Wikipedia article "凌日時間變分法" in Chinese language version.

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arxiv.org

  • Miralda-Escude. Orbital perturbations on transiting planets: A possible method to measure stellar quadrupoles and to detect Earth-mass planets. The Astrophysical Journal. 2001, 564 (2): 1019. Bibcode:2002ApJ...564.1019M. arXiv:astro-ph/0104034可免费查阅. doi:10.1086/324279. 
  • Holman; Murray. The Use of Transit Timing to Detect Extrasolar Planets with Masses as Small as Earth. Science :-,2005. 2004, 307 (1291). arXiv:astro-ph/0412028可免费查阅. doi:10.1106/science.1107822. 
  • Agol; Sari; Steffen; Clarkson. On detecting terrestrial planets with timing of giant planet transits. Monthly Notices of the Royal Astronomical Society. 2004, 359 (2): 567–579. Bibcode:2005MNRAS.359..567A. arXiv:astro-ph/0412032可免费查阅. doi:10.1111/j.1365-2966.2005.08922.x. 
  • Ballard; et. al.; Francois Fressin; David Charbonneau; Jean-Michel Desert; Guillermo Torres; Geoffrey Marcy; Burke; Howard Isaacson. The Kepler-19 System: A Transiting 2.2 R_Earth Planet and a Second Planet Detected via Transit Timing Variations. 2011. arXiv:1109.1561可免费查阅 [astro-ph.EP]. 
  • G.Maciejewski, D.Dimitrov, R.Neuhaeuser, A.Niedzielski, St.Raetz, Ch.Ginski, Ch.Adam, C.Marka, M.Moualla, M.Mugrauer. Transit timing variation in exoplanet WASP-3b. 2010. arXiv:1006.1348v1可免费查阅 [astro-ph.EP]. 
  • M Montalto; et al. A new analysis of the WASP-3 system: no evidence for an additional companion. MNRAS. Nov 2, 2012. arXiv:1211.0218可免费查阅. 

astronomynow.com

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harvard.edu

ui.adsabs.harvard.edu

nasa.gov

kepler.nasa.gov

web.archive.org