An example plot for the global modeling of HD 209458, the first exoplanetary system with RM measurement (D. Queloz et al. 2000). From left to right, each panel represents the fits to the spectral energy distribution (SED), TESS transits, radial velocities, and Rossiter–McLaughlin effects. Figures for all systems can be found at https://github.com/wangxianyu7/Data_and_code/tree/main/e-%CE%BB_Trends.