2 THE SAMI GALAXY SURVEY
2.1 The Sydney AAO Multi-object Integral Field Spectrograph
2.2 Sample Selection and Data Reduction
2.3 LZIFU and Data Products
2.4 Selecting and Characterizing the Sample

3 USING KINEMETRY TO QUANTIFY KINEMATIC ASYMMETRY
3.1 The kinemetry algorithm
3.2 Using kinemetry to measure kinematic asymmetry
3.3 Visually classifying asymmetric galaxies

4 DISTINGUISHING BETWEEN KINEMATICALLY NORMAL AND ASYMMETRIC GALAXIES IN THE SAMI GALAXY SURVEY
4.1 Comparison of the kinemetry technique with quantitative morphology

5 COMPARISON OF OUR RESULTS WITH HIGH REDSHIFT STUDIES

6 THE RELATIONSHIP BETWEEN KINEMATIC ASYMMETRY, COLOUR AND STELLAR MASS

7 STAR FORMATION IN KINEMATICALLY ASYMMETRIC GALAXIES
7.1 Comparison of SAMI Galaxy Survey, SDSS and GAMA SFRs
7.2 Kinematic asymmetry and concentration of star formation
7.3 Kinematic asymmetry and equivalent width of Hα emission
7.4 Possible causes and implications of concentration of star formation

8 KINEMATIC ASYMMETRY OF AGN

9 CONCLUSIONS