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Article Contents
1 Introduction
2 Observational data and standard reduction
3 Additional spectroscopic and photometric processing
4 Integrated canonical modeling of the cluster
5 Need to account for statistical fluctuations
6 Star-by-star characterization of the cluster
7 Discussion
8 Conclusions
References
Online Material
Appendix A: Magnitude interpolation

List of tables
List of figures

Copyright ESO 2004
Published by EDP Sciences