1. Introduction  
2. Observations and Sample Selection  
2.1. Sample Selection  
2.2. VLT/SINFONI Observations and Data Reduction  
2.3. New and Archival VLA Observations  
3. Methodology  
3.1. Integrated Spectra  
3.2. Removal of Nuclear Broad Line Emission  
3.3. Map Construction  
4. Integrated Spectral Properties of the Sample  
4.1. Integrated Spectra  
4.2. Diagnostic Diagrams and Gas-phase Metallicities  
4.3. Electron Densities  
4.4. Extinction and Ionized Gas Masses  
5. Spatially Resolved Properties  
5.1. Continuum Morphologies  
5.2. [OIII] Morphologies and Surface Luminosities  
5.3. Alignment with the Radio Axis  
5.4. Jet and Emission-line Region Sizes and Axis Ratios  
5.5. Comparison of [OIII] λ 5007 and H α Morphologies  
5.6. Emission-line Surface Brightnesses  
6. Gas Kinematics  
6.1. Velocity Patterns and Total Velocity Offsets  
6.2. Line Widths  
6.3. Ratio of Velocity Gradients and Line Widths  
7. Feedback  
7.1. Kinematic Signatures of Rotation?  
7.2. Time Scales  
7.3. Kinetic Jet Power  
7.4. Velocity Range and Estimates from Feedback Models  
7.5. Gas Kinetic Energy and Momentum and Transfer Efficiencies from the Jet to the Gas  
8. Role for Galaxy Evolution  
8.1. Outflows and Turbulence  
8.2. ISM Metal Enrichment  
9. Summary