1. Introduction

2. SDSS-II Supernova Survey Overview
2.1. Imaging
2.2. Supernova Search Pipeline
2.3. Artificial Supernovae
2.4. Spectroscopy
2.5. Final Photometry

3. Defining the SN Ia Sample for the Rate Measurement
3.1. Spectroscopic SN Sample
3.2. Photometric SN Sample

4. Survey Efficiency
4.1. Use of Artificial SN Images
4.2. Monte Carlo Simulations

5. SDSS SN Results
5.1. Volumetric SN Ia rate
5.2. SN Ia Rate per unit galaxy luminosity
5.3. SN Ia Rate as a function of host galaxy type

6. Fitting SN Rate evolution models
6.1. Maximum Likelihood method
6.2. SN Rate Models and Star Formation History
6.3. Rate Measurements: Combining Data Sets
6.4. Fits to SN Ia Rate Models

7. Conclusions