1. Introduction

2. Characterizing the Observational Bias of New CSS

2.1. Photometric Probability of Detection

2.2. Trailing Loss

2.3. Detection Probability as a Function of $a$, $e$, $i$, and $H$

3. NEO Model Parameters and Optimization

4. NEOMOD v2.0

5. A Case for Tidal Disruption

6. Planetary Impacts

7. Discussion