Abstract: I present a measurement of the conditional occurrence of distant giant planets in the presence of close-in small planets, demonstrating that such giants are slightly enhanced over the field rate when they have a small inner neighbor. In January of 2024 I completed the Distant Giants Survey, a 3-year radial velocity (RV) survey to estimate the conditional occurrence of long-period Jupiter analogs in systems hosting small transiting planets. Kepler taught us that small close-in planets occur at a rate of ~1 per Sun-like star. Meanwhile, ground-based RV surveys have shown that long-period gas giants are rarer, with an occurrence rate of ~0.15 per Sun-like star. By searching for giant planets in systems with known close-in small planets, I found that giant planets are more common (~0.3 per star) when a close-in small planet is present. This finding will help to refine exoplanet formation models and determine whether the solar system's architecture is a common outcome of exosystem evolution.