  The Kepler Mission has provided unprecedented, nearly continuous photometric
data of $\sim$200,000 objects in the $\sim$105 deg$^{2}$ field of view from the
beginning of science operations in May of 2009 until the loss of the second
reaction wheel in May of 2013. The Kepler Eclipsing Binary Catalog contains
information including but not limited to ephemerides, stellar parameters and
analytical approximation fits for every known eclipsing binary system in the
Kepler Field of View. Using Target Pixel level data collected from Kepler in
conjunction with the Kepler Eclipsing Binary Catalog, we identify false
positives among eclipsing binaries, i.e. targets that are not eclipsing
binaries themselves, but are instead contaminated by eclipsing binary sources
nearby on the sky and show eclipsing binary signatures in their light curves.
We present methods for identifying these false positives and for extracting new
light curves for the true source of the observed binary signal. For each
source, we extract three separate light curves for each quarter of available
data by optimizing the signal-to-noise ratio, the relative percent eclipse
depth and the flux eclipse depth. We present 289 new eclipsing binaries in the
Kepler Field of View that were not targets for observation, and these have been
added to the Catalog. An online version of this Catalog with downloadable
content and visualization tools is maintained at
http://keplerEBs.villanova.edu.
