1. INTRODUCTION

2. DATA
2.1. Hubble Space Telescope Data
2.2. Additional Photometry
2.3. Near-Infrared Spectroscopy

3. LYMAN CONTINUUM CANDIDATES
3.1. Detections
3.2. Gold and Silver Subsamples
3.3. Spatial Offsets
3.4. Foreground Contamination
3.5. Non-Detections

4. ANALYSIS
4.1. Relative Escape Fractions
4.2. SED Model Fits
4.3. Measured vs. Model Line Fluxes
4.4. Composite SEDs

5. RESULTS
5.1. Dependence on the Strength of Lyα
5.2. Dependence of fesc on Luminosity and Stellar Mass
5.3. Dependence of fesc on the Strength of [O III]

6. DISCUSSION
6.1. Understanding the Non-Detections
6.2. Comparison to Other Studies
6.3. Implications for Cosmic Reionization

7. SUMMARY