1 INTRODUCTION

2 TWO THEORETICAL PILLARS
2.1 Halo Occupation Distribution
2.2 Halo Model

3 MODELLING THE OBSERVABLE
3.1 Correlations Between Galaxy Positions and the Dark Matter Distribution
3.2 Modeling the Tangential Shear
3.3 Tidal Stripping of the Satellites
3.4 Point-Mass Contribution
3.5 Lens Magnification
3.6 Intrinsic Alignment

4 DATA
4.1 Lens Galaxies - redMaGiC
4.2 Lens Galaxies - MagLim
4.3 Source Galaxies

5 MEASUREMENTS

6 MODEL FITTING

7 RESULTS
7.1 Model Fits
7.2 Halo Properties
7.3 Robustness Tests

8 SUMMARY AND DISCUSSION