Spectroscopic GSP-Spec (crosses) and XGBoost (circles) parameters and asteroseismic measurements of the surface gravity (top panel) and masses (bottom panel) of red giant binaries (Beck et al. 2024) and rotational binaries (Gaulme et al. 2020) with solar-like oscillations. The two spectroscopic values are connected with a vertical dashed line. The color bar shows the activity index and the difference in Δlog g in the top and bottom panels, respectively. The median difference and dispersion between spectroscopic and asteroseismic masses are quoted in the bottom panel.