1 INTRODUCTION

2 DYNAMICAL ANALYSIS OF THE DISKMASS SURVEY
2.1 Rotation curve fitting
2.2 Stellar vertical velocity dispersions

3 PRELIMINARY MODELLING
3.1 Bulge-Disk decomposition
3.2 The MOND Poisson solver
3.3 Error budget

4 PRIMARY RESULTS
4.1 Parameter posterior probabilities
4.2 Comparison of the fitted hz vs hR with observations
4.3 Two dimensional Kolmogorov-Smirnov test
4.4 Superposition of M/L distributions
4.5 Why does MOND need such thin disks?
4.6 Central dynamical surface density versus central surface luminosity density

5 SECONDARY RESULTS: VARYING ADDITIONAL PARAMETERS
5.1 Variation of the Stellar Velocity dispersion Ellipsoid
5.2 Fixed scale-height, unconstrained inclination
5.3 Variable MOND acceleration parameter
5.4 Sech² vertical distributions

6 CONCLUSIONS AND DISCUSSION