Inputs required by KOBE to simulate the Kepler transit survey. Left: Distribution of stellar noise, rms CDPP_{6 h}, as seen by Kepler for FGK solar-type stars. Each individual KOBE system is assigned a CDPP value from this distribution. Right: Two-dimensional histogram depicting completeness of Kepler’s Robovetter, as calculated by KOBE-Vetter. To emulatehigh reliability, a disposition score cut-off is placed. Labels on each bin indicate the completeness (in %) for that bin. This calculation is based on the injected transit signals (Coughlin 2017). Completeness is not calculated for bins with less than ten injected signals (not labelled). These bins are assigned a completeness of 0%.