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Planet Detectability in the Alpha Centauri System, , , , и . (2017)cite arxiv:1711.06320Comment: 16 pages, 7 figures, data provided in appendix. Accepted for publication in ApJ.Insights on the Spectral Signatures of Stellar Activity and Planets from PCA, , , , и . (01.08.2017)Formation and Detectability of Terrestrial Planets Around Alpha Centauri B, , , , , и . The Astrophysical Journal, 679 (2): 17 (февраля 2008)Planet Hunters: New Kepler planet candidates from analysis of quarter 2, , , , , , , , , и 7 other автор(ы). (2012)cite arxiv:1202.6007Comment: Submitted to AJ.Improved spectroscopic parameters for transiting planet hosts, , , , , , и . (2012)cite arxiv:1208.1268Comment: 13 pages in emulateapj format, including figures and tables. Accepted for publication in The Astrophysical Journal. The complete tables 5 and 7 will appear in the electronic edition of the Journal.The Planet‐Metallicity Correlation, и . The Astrophysical Journal, 622 (2): 1102--1117 (апреля 2005)Influence of Stellar Multiplicity On Planet Formation. II. Planets Are Less Common in Multiple-Star Systems with Separations Smaller than 1500 AU, , , и . (2014)cite arxiv:1407.3344Comment: 17 pages, 7 figures, 5 tables, accepted by ApJ.Compact multi-planet systems are more common around metal poor hosts, , , и . (2018)cite arxiv:1810.10009Comment: 5 pages, 2 figures, accepted to ApJ Letters.Kepler-20: A Sun-like Star with Three Sub-Neptune Exoplanets and Two Earth-size Candidates, , , , , , , , , и 34 other автор(ы). (2011)cite arxiv:1112.4514Comment: accepted by ApJ, 58 pages, 12 figures revised Jan 2012 to correct table 2 and clarify planet parameter extraction.