1. INTRODUCTION

2. OVERVIEW OF ANALYSIS PROCEDURE

3. OBSERVATIONAL CONSTRAINTS  
3.1. Surface Brightness  
3.2. Velocity Distribution  
3.3. Luminosity Function

4. ANALYSIS  
4.1. Model  
4.2. Model-Data Comparison: Likelihood Function  
4.3. MCMC Sampler

5. RESULTS  
5.1. Confidence Intervals & Correlations  
5.3. Comparison to Previous Measurements  
5.4. Conversion Between Integrated-Light and Star-Count Disk Fractions

6. DISCUSSION  
6.1. Kicked-Up Disk  
6.2. Relationship Between Bulge and Halo  
6.3. Radial Gradient in the Disk LF