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Asteroseismology has the capability of delivering stellar properties whichwould otherwise be inaccessible, such as radii, masses and thus ages of stars.When this information is coupled with classical determinations of stellarparameters, such as metallicities, effective temperatures and angulardiameters, powerful new diagnostics for stellar and Galactic studies can beobtained. The ongoing Stroemgren survey for Asteroseismology and GalacticArchaeology (SAGA) is pursuing such a goal, by determining photometric stellarparameters for stars with seismic oscillations measured by the Keplersatellite. As the survey continues and expands in sample size, SAGA willprovide an unprecedented opportunity to constrain theories of the evolution ofthe Milky Way disc.

The SAGA so far: reading the history of the Galaxy with asteroseismology