Pre-Spectroscopic False Positive Elimination of Kepler Planet Candidates

@article{Batalha2010PreSpectroscopicFP,
  title={Pre-Spectroscopic False Positive Elimination of Kepler Planet Candidates},
  author={Natalie M. Batalha and Jason F. Rowe and Ronald L. Gilliland and Jon M. Jenkins and Douglas A. Caldwell and William J. Borucki and David G. Koch and Jack J. Lissauer and Edward Wood Dunham and Thomas Gautier and Steve B. Howell and David W. Latham and Geoffrey W. Marcy and Andrej Pr{\vs}a},
  journal={The Astrophysical Journal},
  year={2010},
  volume={713}
}
Ten days of commissioning data (Quarter 0) and 33 days of science data (Quarter 1) yield instrumental flux time series of ~150,000 stars that were combed for transit events, termed threshold crossing events(TCE), each having a total detection statistic above 7.1?. TCE light curves are modeled as star+planet systems. Those returning a companion radius smaller than 2RJ are assigned a Kepler Object of Interest (KOI) number. The raw flux, pixel flux, and flux-weighted centroids of every KOI are… 

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