1 INTRODUCTION

2 DETERMINING STELLAR PARAMETERS
2.1 Combining Input Data
2.2 Stellar Masses, Radii, Luminosities, Ages via Isochrones
2.3 Comparison of Stellar Parameter Estimates

3 REFINING PLANETARY SYSTEMS

4 DISCUSSION
4.1 Identifying False Positives
4.2 Follow-up and Mass Confirmation from Ground-Based Surveys
4.3 Planetary Compositions from Mass-Radius Relations
4.4 Chemical Abundances of Confirmed and Candidate Exoplanets
4.5 Assessing the Radius Valley and Super-Earth Desert

5 CONCLUSION