摘要：

We present a catalog of revised effective temperatures for stars observed in long-cadence mode in the Kepler Input Catalog (KIC). We use Sloan Digital Sky Survey (SDSS) griz filters tied to the fundamental temperature scale. Polynomials for griz color-temperature relations are presented, along with correction terms for surface gravity effects, metallicity, and statistical corrections for binary companions or blending. We compare our temperature scale to the published infrared flux method (IRFM) scale for VTJKs in both open clusters and the Kepler fields. We find good agreement overall, with some deviations between (J – Ks )-based temperatures from the IRFM and both SDSS filter and other diagnostic IRFM color-temperature relationships above 6000?K. For field dwarfs, we find a mean shift toward hotter temperatures relative to the KIC, of order 215?K, in the regime where the IRFM scale is well defined (4000?K to 6500?K). This change is of comparable magnitude in both color systems and

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