2 DATA
2.1 Density profiles
2.2 Mass-to-light ratio from SPS models
2.3 Kinematics
2.4 Effect of tracer density profiles on the observed kinematics

3 DYNAMICS: MASS AND ANISOTROPY DISTRIBUTION

4 COMBINING RED AND BLUE GLOBULAR CLUSTER DYNAMICS
4.1 Best-fit halo parameter determination
4.2 Self-consistent models

5 DISCUSSION
5.1 Orbital anisotropies and implications for formation processes
5.2 Dark matter halo properties and IMF
5.3 Comparison with other works

6 CONCLUSIONS