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The raw light curves of both KIC 10684673 and KIC 12216817 show variability.Both are listed in the Kepler Eclipsing Binary Catalog (hereafter KEBC),however both are flagged as uncertain in nature. In the present study we showtheir light curves can be modeled by considering each target as a single,multi-modal delta Scuti pulsator. While this does not exclude the possibilityof eclipsing systems, we argue, while spectroscopy on the systems is stilllacking, the delta Scuti model is a simpler explanation and therefore moreprobable.

Modeling KIC10684673 and KIC12216817 as Single Pulsating Variables