Upper panel: red circles mark the 18 stars in the sample that have exoplanets detected and good Li measurements. Bottom panel: difference between the A(Li) for individual stars to the mean A(Li) for stars that have no exoplanet detections and that have effective temperatures, surface gravities, and metallicities, within ±75 K, ±0.2 dex, and ±0.2 dex. For stars with T_eff > 6100 K, the temperature range is expanded to ±200 K.