1 INTRODUCTION
2 DATA AND METHODS
2.1 Data Reduction and Sample
2.2 Galaxy Kinematics
2.3 Galaxy Morphologies
3 SAMI SCALING RELATIONS
3.1 $S_{0.5}$ Reduces Scatter
3.2 Linearity of the $S_{0.5}$ Scaling Relation
3.3 Effect of Spaxel-Level Quality Cut
3.4 Gas and Stellar $S_{0.5}$ Disagreement
3.5 IFS and Aperture Kinematic Measurements
3.6 Comparing IFS and Aperture Scaling Relations
3.7 Varying $K$
4 DISCUSSION
4.1 SAMI Scaling Relations
4.2 IFS and Aperture Kinematics
4.3 The Importance of $K$
5 CONCLUSIONS