VALIDATION OF KEPLER'S MULTIPLE PLANET CANDIDATES. III. LIGHT CURVE ANALYSIS AND ANNOUNCEMENT OF HUNDREDS OF NEW MULTI-PLANET SYSTEMS

@article{Rowe2014VALIDATIONOK,
  title={VALIDATION OF KEPLER'S MULTIPLE PLANET CANDIDATES. III. LIGHT CURVE ANALYSIS AND ANNOUNCEMENT OF HUNDREDS OF NEW MULTI-PLANET SYSTEMS},
  author={Jason F. Rowe and Stephen T. Bryson and Geoffrey W. Marcy and Jack J. Lissauer and Daniel Jontof-Hutter and Fergal Robert Mullally and Ronald L. Gilliland and Howard Issacson and Eric B. Ford and Steve B. Howell and William J. Borucki and Michael Haas and Daniel Huber and Jason H. Steffen and S. Thompson and Elisa V. Quintana and Thomas Barclay and Martin D. Still and Jonathan J. Fortney and Thomas Gautier and Roger C. Hunter and Douglas A. Caldwell and D R DeVore and William D. Cochran and Jon M. Jenkins and Eric Agol and Joshua A. Carter and John Charles Geary},
  journal={The Astrophysical Journal},
  year={2014},
  volume={784},
  pages={45}
}
The Kepler mission has discovered more than 2500 exoplanet candidates in the first two years of spacecraft data, with approximately 40% of those in candidate multi-planet systems. The high rate of multiplicity combined with the low rate of identified false positives indicates that the multiplanet systems contain very few false positive signals due to other systems not gravitationally bound to the target star. False positives in the multi-planet systems are identified and removed, leaving behind… 
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