1 INTRODUCTION
2 OBSERVATIONS AND DATA REDUCTION
3 LOCATION OF THE OBSERVED STAR CLUSTERS
3.1 De projected distance to the LMC centre
3.2 Clusters distance to the SMC centre
4 CLUSTER STRUCTURES FROM EMPIRICAL MODEL FITTINGS
4.1 Model fittings to radial density profiles
4.2 Model fittings to surface brightness profiles
4.3 Integrated absolute $V$ magnitude
4.4 Comparison with previous studies
4.5 Assessing the fit quality
5 STRUCTURAL PARAMETERS AND THEIR SPATIO-TEMPORAL DISTRIBUTION
5.1 Spatial properties
5.2 Structure versus age
5.3 Mass distribution
6 HALF-LIGHT AND JACOBI RADII
7 DISCUSSION