1. INTRODUCTION

2. SINS SAMPLE SELECTION
2.1. Optically-Selected BX/BM Objects
2.2. Near-/Mid-IR-Selected Galaxies
2.3. Lyman-Break Galaxies
2.4. Submillimeter-Bright Galaxies
2.5. Line Emitters

3. GALAXY POPULATIONS PROBED BY THE SINS Hα SAMPLE

4. SINFONI OBSERVATIONS
4.1. SINFONI Observations
4.2. SINFONI Data Reduction

5. EXTRACTION OF EMISSION LINE AND KINEMATIC PROPERTIES
5.1. Line Emission and Kinematics Maps
5.2. Integrated Spectra and Properties
5.3. Axis Profiles and Position-Velocity Diagrams
5.4. Size Estimates

6. INTEGRATED Hα PROPERTIES OF THE SINS Hα SAMPLE
6.1. Hα Detections and Flux Sensitivity Limits
6.2. Distributions of Hα Fluxes, Velocity Dispersions, and Sizes
6.3. Impact of Sensitivity Limits and Observing Strategy on Trends with Hα Velocity Dispersions and Sizes

7. COMPARISON WITH OTHER $Z\sim2$ SPECTROSCOPIC SAMPLES
7.1. Comparison with the NIRSPEC BX/BM Sample
7.2. Comparison with Other IFU Samples

8. DUST DISTRIBUTION AND STAR FORMATION PROPERTIES
8.1. Intrinsic Hα Luminosities, Hα Equivalent Widths, and Star Formation Rates Estimates
8.2. Constraints on the Dust Distribution
8.3. Constraints on the Star Formation Histories
8.4. Star Formation Rate Estimates

9. SPATIALLY-RESOLVED Hα KINEMATICS AND KINEMATIC DIVERSITY
9.1. Kinematic Classification
9.2. Rotation-Dominated High Redshift Galaxies
9.3. Dispersion-Dominated High Redshift Galaxies
9.4. Merger/Interacting High Redshift Systems
9.5. Dynamical versus Evolutionary State
9.6. Mass Fractions and Constraints on Dark Matter Contribution

10. SUMMARY