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Solar-like oscillating giants observed by the space-borne satellites CoRoTand Kepler can be used as key tracers of stellar populations in the Milky Way.When combined with additional photometric/spectroscopic constraints, thepulsation spectra of solar-like oscillating giant stars not only reveal theirradii, and hence distances, but also provide well-constrained estimates oftheir masses, which can be used as proxies for the ages of these evolved stars.In this contribution we provide supplementary material to the comparison wepresented in Miglio et al. (2013) between populations of giants observed byCoRoT in the fields designated LRc01 and LRa01.

Differential population studies using asteroseismology: solar-like oscillating giants in CoRoT fields LRc01 and LRa01