Four top panels show the delayed eccentricities for super-Jupiter systems starting in the 2:1-2:1 configuration. From top to bottom the set of planetary masses are (1.5, 2, 2.5) m_Jup, (2.25, 3, 3.75) m_Jup, (3, 4, 5) m_Jup and (3.75, 5, 6.25) m_Jup. Colors and markers follow the scheme used in Figure 4. The bottom panel shows the CDF for the distances of the flyby, each curve represents a different mass configuration.