Orbital range of outermost super-Earth and innermost cold Jupiter plotted by host star metallicity. For each system, we plot the orbital range (periapsis to apoapsis) of the outermost super-Earth (red) and innermost cold Jupiter (yellow). Cold Jupiters in systems without super-Earths are shown in blue, and light markers correspond to giant planets that did not survive. Cold Jupiter systems with host star metallicities greater than ~ 0.3 typically harbor no super-Earths, and high-metallicity giants without super-Earths are often on eccentric orbits.