1. Introduction

2. MegaPrime and MegaCam

3. The SNLS Survey

4. Photometry
4.1. Aperture Photometry
4.2. Background Estimation
4.3. Aperture Corrections

5. The Elixir Pipeline
5.1. Plate Scale Variations
5.2. Elixir Strategy

6. The Photometric Grids
6.1. The Photometric Response Maps
6.2. Measuring the Photometric Response Maps
6.3. Monte-Carlo Checks
6.4. Results
6.5. Comparison with Elixir Findings
6.6. Applying the Grid Corrections to the Data

7. MegaCam Passbands
7.2. Effective Passbands
7.3. Comparison of the Observed and Synthetic Color Terms

8. Landolt Stars
8.1. The Landolt Photometric System
8.2. Calibration Model
8.3. Results

9. MegaCam Magnitudes
9.1. Uniform Magnitudes
9.2. Local Natural Magnitudes

10. Flux Interpretation of the MegaCam Magnitudes
10.1. Selecting a Fundamental Standard
10.2. The MegaCam Magnitudes of BD+17 4708

11. Tertiary Catalogs
11.1. Tertiary Star Selection
11.2. Building the Tertiary Catalogs
11.3. Photometric Error Model
11.4. Outlier Rejection
11.5. Photometric Night Selection
11.6. Results
11.7. Statistical Uncertainties

12. Systematic Uncertainties
12.1. Photometry Related Errors
12.2. The Airmass Corrections
12.3. The Shutter Precision
12.4. Landolt Catalog Internal Dispersion
12.5. Grid Reference Colors
12.6. Adequacy of the Grid Color Corrections
12.7. The Magnitudes of BD+17 4708
12.8. The SED of BD+17 4708
12.9. Summary: the Full Uncertainty Budget

13. Discussion