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Exoplanetary transits produce a double-horned color signature that isdistinct from both binaries and blends and can thus be used to separateexoplanets from false positives in transit searches. Color photometry withprecision sufficient to detect this signal in transits of HD 209458 isavailable in the literature. Analysis of these observations reveals that, whilethe signature does exhibit the expected shape, it is significantly strongerthan PHOENIX atmospheric models predict.Comment: 4 pages, 3 figures, accepted to A&

The color signature of the transit of HD 209458: discrepancies between stellar atmospheric models and observations