1 INTRODUCTION
2 RAW TRANSIENT DATA
2.1 Survey Overview
2.2 Candidate-Observation Quality Filtering
2.3 Sample Quality Assessment
3 KNOWN-OBJECT EXTRACTION
3.1 Implementation of KD-tree Indexing
3.2 Matching Ephemerides Against the KD-tree
3.3 Summary of Known Small-Bodies Detected
3.4 Overlap of PTF with the WISE and SDSS Data Sets
4 UNKNOWN-OBJECT EXTRACTION
4.1 Previous and Ongoing PTF Small-Body Discovery Work
4.2 A Custom Discovery Algorithm for Main-Belt Objects
4.3 Summary of Objects Discovered
5 EXTENDED-OBJECT ANALYSIS: APPROACH
5.1 Definition of the Extended Ness Parameter $\mu$
5.2 Systematic (Non-Cometary) Variation in $\mu$
5.3 Formalism for Interpreting $\mu$
5.4 A Model $\mu$ to Describe Inert Objects
5.5 Defining a Visually-Screenable Sample
6 EXTENDED-OBJECT ANALYSIS: RESULTS
6.1 A New Quasi-Hilda Comet: 2011 $\mathbf{CR}_{42}$
7 STATISTICAL INTERPRETATION
7.1 Bayesian Formalism
7.2 Active MBCs in the Entire Main-Belt
7.3 Active MBCs in the Outer Main-Belt
7.4 Active MBCs in the Low-Inclination Outer Main-Belt
7.5 Active MBCs Among Low $i$ Outer Main-Belt Objects Observed Near Perihelion $(-45^{\circ}<\nu<45^{\circ})$
7.6 Active MBCs in the Sub Diameter Population
7.7 Active MBCs Among Low-Albedo (WISE-Sampled) Objects
7.8 Active MBCs Among C-Type (SDSS-Sampled) Objects
8 CONCLUSION
8.1 Summary
8.2 Comparison to Previous Work
8.3 Future Work: Photometric (Absolute Magnitude) Variation as a Function of Orbital Anomaly