1. INTRODUCTION

2. THEORETICAL BACKGROUND  
2.1. Galaxy-Mass Power Spectrum  
2.2. Intrinsic Alignment Model  
2.3. Galaxy Angular Power Spectrum

3. DATA  
3.1. Deep Lens Survey  
3.2. Lens and Source Selection  
3.3. Shear Calibration and Tangential Shear Measurement  
3.4. Galaxy Angular Correlation Measurement

4. RESULTS  
4.1. Power Spectrum Reconstruction  
4.2. Covariance Estimation

5. DISCUSSION  
5.1. Comparison of the DLS $S_{8}$ Measurement with Other Studies  
5.2. Impacts of Assumed Cosmology on Parameter Estimation  
5.3. Constraints on Baryonic Feedback Parameter and Model Selection

6. SUMMARY AND CONCLUSIONS