Correlations with the dust flux after 1 Gyr of dynamical and collisional evolution for the seeds simulations, as compared with the mixed simulations. The top panels show F/F_star at 70   μm vs. the eccentricity of the innermost surviving giant planet (left) and the total mass in surviving terrestrial planets (right). The bottom panels show the same comparisons but at 25   μm. The mixed simulations are in black, the smallseed simulations in green, and the bigseed simulations in red. Filled circles represent stable simulations and open circles unstable simulations.