1. INTRODUCTION

2. THE MODEL

3. THE BAYESIAN SETUP  
3.1. Constraints  
3.2. Likelihood  
3.3. Prior  

4. RESULTS  
4.1. Nuclear matter  
4.2. Neutron stars matter  
4.3. Model dependence of the results  
4.4. Correlations between parameters of NM  
4.5. Correlations between parameters of NM and properties of NSs  

5. SUMMARY  

6. CONCLUSIONS