Cumulative distribution of the eccentricity (top), masses (middle) and semi-major axes (bottom) of giant planets with orbital distances of up to 5 AU and masses above 0.5 Jupiter masses, separated into systems with (red line) and without (blue line) inner sub-Neptunes. We merged here all the data of the simulations with κ = 0.3 cm² g⁻¹, κ = 0.4 cm² g⁻¹ and κ = 0.4 cm² g⁻¹ with S_peb = 10.0.