1 INTRODUCTION

2 DATA  
2.1 Dark Energy Survey Observations  
2.2 Dark Energy Survey Shear Catalogs  
2.3 South Pole Telescope Observations  
2.4 SZE Selected Lens Sample  

3 CLUSTER SHEAR PROFILES  
3.1 Background Source Selection  
3.2 Cluster Member Contamination  
3.3 Assumed Cluster Profile  
3.4 Radial Fitting Range and Binning  
3.5 Calibration of WL Mass Bias and Scatter  

4 SCALING RELATION ANALYSIS  
4.1 Bayesian Forward Modeling Framework  
4.2 Priors  
4.3 Results for $\zeta-M_{500}$ Scaling Relation  
4.4 Comparison to Previous Results  

5 CONCLUSIONS