1. INTRODUCTION

2. SURVEY OVERVIEW  
2.1. Target Selection  
2.2. Observing Strategy  
2.3. Science Images  
2.4. Template Images  
2.6. Redshifts  
2.7. Classification  

3. DATA REDUCTION  
3.1. Validating Image Subtraction  
3.2. Repeatability of Stellar Magnitudes  

4. CALIBRATION  
4.1. Calibration Zeropoints for each Image  

5. LIGHT CURVE MODEL DESCRIPTIONS AND FITS  
5.2. SNooPy  
5.3. BayeSN  

6. HUBBLE DIAGRAM

7. DISCUSSION

8. CONCLUSIONS