ARCHITECTURE AND DYNAMICS OF KEPLER'S CANDIDATE MULTIPLE TRANSITING PLANET SYSTEMS

@article{Lissauer2011ARCHITECTUREAD,
  title={ARCHITECTURE AND DYNAMICS OF KEPLER'S CANDIDATE MULTIPLE TRANSITING PLANET SYSTEMS},
  author={Jack J. Lissauer and Darin Ragozzine and Daniel C. Fabrycky and Jason H. Steffen and Eric B. Ford and Jon M. Jenkins and Avi Shporer and Matthew J. Holman and Jason F. Rowe and Elisa V. Quintana and Natalie M. Batalha and William J. Borucki and Stephen T. Bryson and Douglas A. Caldwell and Joshua A. Carter and David R. Ciardi and Edward Wood Dunham and Jonathan J. Fortney and Thomas Gautier and Steve B. Howell and David G. Koch and David W. Latham and Geoffrey W. Marcy and Robert C. Morehead and Dimitar D. Sasselov},
  journal={The Astrophysical Journal Supplement Series},
  year={2011},
  volume={197}
}
About one-third of the ∼1200 transiting planet candidates detected in the first four months of Kepler data are members of multiple candidate systems. There are 115 target stars with two candidate transiting planets, 45 with three, 8 with four, and 1 each with five and six. We characterize the dynamical properties of these candidate multi-planet systems. The distribution of observed period ratios shows that the vast majority of candidate pairs are neither in nor near low-order mean-motion… 

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