can be inferred from current data. RV+Kepler data are well explained as a single population with xl ≈ 2. For HAT+WASP data... 85% consistent with high-e migration history 15% consistent with disk migration history Caveats including but not limited to: 1. NASA Exoplanet Archive query missed some planets due to filtering issues; 2. similar analysis with exoplanets.org data show moderately different constraints on some pop-level parameters; 3. smaller sample size for RV and Kepler, more data could reveal 1<x<2 planets in these datasets; 4. we only include data on x, nothing on obliquity, additional companions, etc.; 5. unclear if HAT and WASP have significant observing biases affecting shape of x distribution; 6. large asymmetries in planet radius estimates not accurately modeled with Gaussian; 7. hard edge most sensitive to planet with smallest x, doesn’t offer enough flexibility for outliers * *