1. INTRODUCTION

2. DATA

2.1. NGDEEP Imaging and Photometry

3. METHODOLOGY

3.1. Galaxy Sample

3.2. Deriving the UV spectral slope from SED fitting

3.3. Deriving the UV spectral slope, β, from photometric power-law fitting

3.4. Literature Comparison Samples

4. RESULTS

4.1. Highlighting Six Example Galaxies

4.2. Verifying our methodology with simulations

5. DISCUSSION

5.1. Modeling caveats

5.2. Comparison with previous work

5.3. Comparison to model predictions

5.4. Implications

6. CONCLUSIONS