1. Introduction

2. Summary of Observations and Data Reduction

3. Transit Selection Pipeline
3.1. Light Curve Post-Processing
3.2. Transit Selection

4. Transit Candidates
4.1. Discussion of Individual Transit Candidates

5. Transit Detection Efficiency Calculation
5.1. Cluster Members
5.2. Field Stars

6. Results
6.1. Cluster Members
6.2. Field Stars
6.3. Errors on the Upper Limits
6.4. Comparison with Previous Results
6.5. Expected Planet Yield

7. Discussion