1. Introduction

2. Instrument suite
2.1. General features
2.2. Filter set

3. Characteristics of the supernova survey

4. Methodology
4.1. Point source photometry
4.2. Light curve fitter training
4.3. Fisher Matrix
4.4. Cosmological priors

5. Results

6. Discussion
6.1. Comparison with weak shear performance
6.2. Summary