1 INTRODUCTION
1.1 Background
2 DATA
2.1 SAMI Galaxy Survey
2.2 Ancillary data
3 METHOD
3.1 Stellar populations
3.2 Kinematics
3.3 Line fitting
3.4 Completeness
4 RESULTS
4.1 Kinematic classification
4.2 Global relations
4.3 Slow rotators
4.4 Relations for the quenched sample
5 DISCUSSION
5.1 Comparisons to previous studies
5.2 Physical implications
6 CONCLUSIONS