Comparison between asteroseismic parameter estimates and the Gaia-FLAME values. Left: Stellar mass estimate from our analysis. It is mostly consistent with the FLAME pipeline. However, there is a slight systematic offset to lower masses in our analysis. Centre: Most radii agree between the two methods, while some outliers with large radii from the asteroseismic analysis can be found. These stars typically have a higher asteroseismic age and are more evolved in our analysis. Right: Additional asteroseismic information from Π₀ gives a good handle on the stellar age. Consequently, we observe a large scatter and a larger spread in age compared to Gaia-FLAME.