2 THE WFCAM TRANSIT SURVEY

3 PIPELINE OVERVIEW

4 A SAMPLE OF M DWARFS
4.1 Identification of M dwarfs
4.2 Interstellar extinction
4.4 M Dwarf Lightcurves
4.5 The WTS sample compared to other surveys
4.6 A lack of hot Jupiters discovered around M dwarfs in the WTS

5 SIMULATION METHOD
5.1 Recovery ratio
5.2 Determining P_r

6 RESULTS AND DISCUSSION
6.1 Sensitivity effect of the observation strategy
6.2 Detection statistic
6.3 Detected period
6.4 False positives
6.5 Transit recovery ratios
6.6 Error considerations
6.7 Limits on planetary fraction

7 DISCUSSION: COMPARISON WITH KEPLER AND RV STUDIES
7.1 Comparison with RV studies

8 SUMMARY