Eccentricity and semi-major axes of the planets in each system of simulation 4f_long at a randomly picked time for each system in each phase. From top to bottom we show the cases of 1-, 2-, 3-, and 4-planet systems and from left to right we show phase A, B, and C. All phase A systems have low eccentricity and four planets. In phase B, the systems have three or more planets. Typically, systems in phase C have two planets, one at a ~ 10 AU and one at 30 ≲ a ≲ 1000 AU. Both phase B and C show generally higher eccentricities.