1. INTRODUCTION

2. DATA SETS
2.1. Selection Requirements
2.2. SNLS SNe
2.3. Low-z SNe
2.4. HST SNe
2.5. SDSS SNe
2.6. U-band Observations of Nearby SNe
2.7. Selection Effects for External Samples
2.8. Peculiar Velocities

3. COSMOLOGICAL RESULTS AND STATISTICAL UNCERTAINTIES WITH THE COMBINED SN SAMPLE
3.1. Model for Relative Distance Moduli
3.2. Correcting for Host-galaxy Properties
3.3. Combining SALT2 and SiFTO
3.4. Statistical Results

4. COSMOLOGICAL RESULTS INCLUDING SYSTEMATIC UNCERTAINTIES
4.1. Systematics Methodology
4.2. Light-curve Training
4.3. Method for Presenting Systematic Effects
4.4. Combined Statistical and Systematic Results
4.5. Tension Between Data Sets
4.6. The Consequences of Simplified Treatments

5. INDIVIDUAL SYSTEMATIC TERMS
5.1. Calibration
5.2. Comparisons of Different Light-Curve Fitters
5.3. Peculiar Velocities, z_cut, and the "Hubble Bubble"
5.4. Malmquist Bias
5.5. Contamination by Other Types of SNe in the SNLS Sample
5.6. Milky-Way Extinction Correction
5.7. Evolution
5.8. Environmental Dependence of SN Properties
5.9. Gravitational Lensing

6. COMPARISON OF UNCERTAINTY BUDGET WITH OTHER ANALYSES

7. HOW THESE SYSTEMATICS WILL BE REDUCED

8. CONCLUSIONS