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The Kepler Input Catalog (KIC) provides reddening estimates for its stars,based on the assumption of a simple exponential dusty screen. This projectfocuses on evaluating and improving these reddening estimates for the KIC'sgiant stars, for which extinction is a much more significant concern than forthe nearby dwarf stars. We aim to improve the calibration (and thusconsistency) amongst various photometric and spectroscopic temperatures ofstars in the Kepler field by removing systematics due to incorrect extinctionassumptions. The revised extinction estimates may then be used to deriveimproved stellar and planetary properties. We plan to eventually use the largenumber of KIC stars as probes into the structure and properties of the GalacticISM.

Preliminary Evaluation of the Kepler Input Catalog Extinction Model Using Stellar Temperatures