  Core overshoot is a large source of uncertainty in constructing stellar
models. Whether the amount of overshoot is constant or mass dependent is not
completely known, even though models sometimes assume a mass-based trend. In
this work we use asteroseismic data from stars observed by \textit{Kepler} to
investigate the relationship between various stellar properties and the amount
of overshoot needed to properly model a given star. We find a strong positive
trend between stellar mass and overshoot amount for stars between 1.1 and 1.5
$M_\odot$, with a slope of 0.89. Additionally, we investigate how inferred
stellar properties change as a function of overshoot. Our model grids show that
the inferred stellar mass and radius can vary by as much as 14\% and 6\%
respectively, depending on the extent of overshoot. This mass spread results in
a commensurate spread in the ages.
