Recently the number of main-sequence and subgiant stars exhibiting solar-like oscillations that are resolved
into individual mode frequencies has increased dramatically. While only a few such data sets were available
for detailed modeling just a decade ago, the Kepler mission has produced suitable observations for hundreds
of new targets. This rapid expansion in observational capacity has been accompanied by a shift in analysis
and modeling strategies to yield uniform sets of derived stellar properties more quickly and easily. We use
previously published asteroseismic and spectroscopic data sets to provide a uniform analysis of 42 solar-type
Kepler targets from the Asteroseismic Modeling Portal (AMP). We find that fitting the individual frequencies
typically doubles the precision of the asteroseismic radius, mass and age compared to grid-based modeling of
the global oscillation properties, and improves the precision of the radius and mass by about a factor of three
over empirical scaling relations. We demonstrate the utility of the derived properties with several applications
