THE KEPLER-19 SYSTEM: A TRANSITING 2.2 R ⊕ PLANET AND A SECOND PLANET DETECTED VIA TRANSIT TIMING VARIATIONS

@article{Ballard2011THEKS,
  title={THE KEPLER-19 SYSTEM: A TRANSITING 2.2 R ⊕ PLANET AND A SECOND PLANET DETECTED VIA TRANSIT TIMING VARIATIONS},
  author={S. Ballard and D. Fabrycky and F. Fressin and D. Charbonneau and J. D{\'e}sert and G. Torres and G. Marcy and C. Burke and H. Isaacson and C. Henze and J. Steffen and D. Ciardi and S. Howell and W. Cochran and M. Endl and S. Bryson and J. Rowe and M. Holman and J. Lissauer and J. Jenkins and M. Still and E. Ford and J. Christiansen and C. Middour and M. R. Haas and J. Li and Jennifer R. Hall and S. McCauliff and N. Batalha and D. Koch and W. Borucki},
  journal={The Astrophysical Journal},
  year={2011},
  volume={743},
  pages={200}
}
We present the discovery of the Kepler-19 planetary system, which we first identified from a 9.3 day periodic transit signal in the Kepler photometry. From high-resolution spectroscopy of the star, we find a stellar effective temperature T_(eff) = 5541 ± 60 K, a metallicity [Fe/H] = –0.13 ± 0.06, and a surface gravity log(g) = 4.59 ± 0.10. We combine the estimate of T_(eff) and [Fe/H] with an estimate of the stellar density derived from the photometric light curve to deduce a stellar mass of M_… Expand
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