(A) Effective temperature (T_eff) versus apparent V magnitude for the stars in the TESS simulation. (B) Orbital period versus planetary radius for all planets in the TESS simulation, whether or not they were detected by TESS. (C) T_eff versus apparent V magnitude for the stars included in our APR RV follow-up program (V < 11, T_eff < 6000 K, and decl. >− 15). (D) Orbital period versus planetary radius for planets orbiting stars meeting our selection criteria for the APF, whether or not they were detected by TESS, plus the true Jupiter analogs we add around 3% of the simulation stars.