1. Introduction

2. Observations

3. Analysis method
3.1. Stellar parameters and atmospheric models
3.2. Line selection and atomic data

4. Abundance results
4.1. Li and CNO
4.2. Sodium to titanium
4.3. Iron group elements and Zn
4.4. Heavy elements
4.5. Error budget

5. Comparison to other r-II stars and Solar r-process abundances

6. Age determination

7. Conclusions