1 INTRODUCTION  
2 DATA SOURCES  
2.1 MaNGA & Pipe3D  
2.2 SDSS Ancillary Data & Sample Selection  
3 METHODS  
3.1 Global Star Formation Metrics  
3.2 Local Star Formation Metrics  
3.3 Radial Profiles  
4 RESULTS FROM RADIAL PROFILES  
4.1 Insights from Population Averaged Profiles  
4.2 Insights from Individual Galaxy Profiles  
5 RANDOM FOREST ANALYSIS - WHICH PARAMETERS MATTER FOR QUENCHING CENTRALS AND SATELLITES?  
5.1 Random Forest Method  
5.2 Random Forest Results  
6 DISCUSSION - HOW DO CENTRAL AND SATELLITE GALAXIES QUENCH?  
6.1 Comparing Central & Satellite Galaxy Quenching  
6.2 Interpretation of the Importance of σc  
6.3 The Role of Black Hole Mass  
6.4 The Role of Halo Mass  
6.5 The Role of Local Galaxy Over-Density  
7 SUMMARY