1. INTRODUCTION
1.2. Mass-Radius Relations
1.3. Motivating Questions for This Work

2. DESCRIPTION OF SURVEY
2.1. Target Selection
2.2. Cadence Choice for RV Observations

3. UNIFORM DETERMINATION OF PLANET RADII
3.1. TESS Light Curve Generation
3.2. Transit Fitting

4. UNIFORM DETERMINATION OF PLANET MASSES
4.1. Radial Velocity Data
4.2. juliet
4.3. Radial Velocity Modeling to Derive Masses to Compare to Literature Values
4.4. Caveats to RV Fitting

5. POPULATION ANALYSIS OF THE MASS-RADIUS RELATION
5.1. Framework: Hierarchical Bayesian Model
5.2. Preliminary M-R Relation with Mid-Survey Masses
5.3. Analysis Including Masses Derived from Literature Values
5.4. Beyond the Single Power Law M-R Relation

6. DISCUSSION
6.1. Comparison of Mass-Radius Relations
6.2. Implications of Planet Compositions from this Study
6.3. Limitations of this Study
6.4. Future Work

7. SUMMARY