Kepler-18b, c, and d: A System of Three Planets Confirmed by Transit Timing Variations, Light Curve Validation, Warm-Spitzer Photometry, and Radial Velocity Measurements
We report the detection of three transiting planets around a Sun-like star, which we designate Kepler-18. The transit signals were detected in photometric data from the Kepler satellite, and were confirmed to arise from planets using a combination of large transit-timing variations (TTVs), radial ve...
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Veröffentlicht in: | The Astrophysical journal. Supplement series 2011-11, Vol.197 (1), p.7-jQuery1323919489348='48' |
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Sprache: | eng |
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