1 INTRODUCTION  
2 SURVEY DESIGN AND TARGET SELECTION  
2.1 Target Selection  
3 DATA ACQUISITION  
3.1 Observations and Data Reduction  
3.2 LOS Velocity Determination  
3.3 Gaia Cross-matching  
4 ISOLATING MAGELLANIC STARS  
5 RESULTS  
5.1 LMC Disk motions  
5.2 Asymmetric LOS Velocity Distributions  
5.3 LMC Mass estimate  
6 SUMMARY