1. INTRODUCTION

2. SAMPLE AND DATA
2.1. Sample Selection
2.2. GBT Observations and Data Reduction
2.3. Ancillary UV, Optical, Infrared, and Radio Data

3. PHOTOMETRY AND ANALYSIS
3.1. GBT Observations: Additional Considerations
3.2. Ancillary Data
3.3. Star Formation Rate Calibrations

4. RESULTS
4.1. Radio Spectral Indices and Estimates for the Thermal Fraction at 33 GHz
4.2. Comparison with 24 µm Warm Dust Emission
4.3. Comparison with Hα and 24 µm Emission
4.4. Comparison with Total IR and UV Emission

5. DISCUSSION
5.1. Dust-Dependent Star Formation Rates
5.2. Variations on the Thermal Fraction and Non-Thermal Spectral Index
5.3. Anomalous Dust Candidates
5.4. The Nascent Starburst NGC 1377

6. CONCLUSIONS