1 INTRODUCTION
2 OBSERVATIONS AND DATA REDUCTION
2.1 X-Shooter and Target Selection
2.2 Data Reduction
3 DETERMINING THE DISTANCE AND STELLAR PARAMETERS
3.1 Temperature and Surface Gravity Determination
3.2 Photometry Fitting
3.3 Mass, Age, Radius, and Log(g) Determination
4 BALMER EXCESS MEASUREMENTS
4.1 Method 1 – Spectral Matching: Single Point Measurement
4.2 Method 2 – B-Band Normalised, Multi-point Measurements
4.3 Comparisons and Checks
5 ACCRETION RATES
5.1 Magnetospheric Modelling
5.2 Literature Comparisons
6 DISCUSSION
6.1 Overall Results
6.2 HR-diagram
6.3 Age
6.4 Accretion Rate vs. Stellar Parameters
7 CONCLUSIONS AND FINAL REMARKS