  Asteroseismology has the capability of delivering stellar properties which
would otherwise be inaccessible, such as radii, masses and thus ages of stars.
When this information is coupled with classical determinations of stellar
parameters, such as metallicities, effective temperatures and angular
diameters, powerful new diagnostics for stellar and Galactic studies can be
obtained. The ongoing Stroemgren survey for Asteroseismology and Galactic
Archaeology (SAGA) is pursuing such a goal, by determining photometric stellar
parameters for stars with seismic oscillations measured by the Kepler
satellite. As the survey continues and expands in sample size, SAGA will
provide an unprecedented opportunity to constrain theories of the evolution of
the Milky Way disc.
