Comparison between the current values for T_eff and log g (x-axis) and those from KSPC DR25 (y-axis) for the Sun-like sample. Δ T_eff and Δ log g correspond to the difference between previous and current constraints. The data points are colored according to their ⟨S_ph⟩. The dashed lines mark the 1-1 lines and the zero difference. The blue shaded region marks the T_eff interval we consider in this study to select Sun-like stars.