1 INTRODUCTION

2 OBSERVATIONS & DATA REDUCTION
2.1 Correlated noise correction

3 ANALYSIS METHODS
3.1 Telluric Correction
3.2 Possible contamination from the 4LGSF
3.3 Stellar & orbital parameters
3.4 Post processing and cross correlation
3.5 Model spectra and cross correlation templates
3.6 CLV+RM modeling
3.7 Narrow-band transmission spectroscopy

4 RESULTS
4.1 Transmission spectra
4.2 Cross correlation analysis

5 DISCUSSION
5.1 Chromatic Rossiter-McLaughlin (CRM)
5.2 Reanalysis of low-resolution WASP-19b transmission spectra

6 SUMMARY AND CONCLUSIONS