1. INTRODUCTION

1.2. Constraining the Abundance of Free-Floating Planets with Roman

2. SIMULATIONS

2.1. Detection Criteria

3. LIGHTCURVES OF FREE-FLOATING PLANETS AS SEEN BY ROMAN

4. PREDICTED YIELDS AND LIMITS

4.2. Limits

5. DISCUSSION

5.1. Event Detection

5.2. False Positives

5.3. Degeneracies

5.4. Wide-bound Confusion

5.5. Limb Darkening and Wave Optics

5.6. Mass Measurements

6. CONCLUSION