1. INTRODUCTION AND SCIENTIFIC MOTIVATION
1.1. SLUGGS
1.2. Survey Comparisons
1.3. This Paper

2. GALAXY SAMPLE SELECTION AND PROPERTIES

3. DATA ACQUISITION, REDUCTION, AND ANALYSIS
3.1. Imaging and Photometry
3.2. Spectroscopy

4. MODELING
4.1. Globular Clusters
4.2. Stellar Properties
4.3. Galaxy Dynamics and Masses

5. MAIN SCIENCE QUESTIONS AND EARLY RESULTS
5.1. Evidence for Two-Phase Galaxy Assembly
5.2. Distinct Subpopulations in GC Systems
5.3. The Nature of Ultra-Compact Dwarfs
5.4. New Constraints on Globular Cluster Formation

6. CONCLUSIONS