1. INTRODUCTION

2. OBSERVATIONAL DETAILS  
2.1. CANDELS  
2.2. CLASH  
2.3. Image Processing, SN Detection, and Classification

3. DETERMINING VOLUMETRIC RATES  
3.1. Observed Number of Events  
3.2. The Control Time  
3.3. CCSN Types  
3.4. K-Corrections  
3.5. Extinction Correction  
3.6. Gravitational Lensing Degradation of the Luminosity Function

4. RESULTS  
4.1. Systematic Errors in CANDELS+CLASH Rates  
4.2. Comparisons to Other CCSN Rates  
4.3. Comparison to Cosmic Star Formation Rate Densities  
4.4. Comparison of Initial Mass Functions

5. SUMMARY