1. INTRODUCTION  
1.1. Extracting the information  

2. METHOD  
2.1. VESPA’s bins  
2.2. SSP Modeling  
2.3. Mock galaxies and wavelength range  

3. DATA  
3.1. Quality of the fits  

4. THE CATALOGUE  
4.1. Masses and mass fractions  
4.2. Error estimates  
4.3. Mass and metallicity per age bin  
4.4. Dust  

5. THE DATABASE  
5.1. Example queries  

6. RESULTS  
6.1. Number of parameters  
6.2. Stellar masses in DR7  
6.3. Metallicity estimates  
6.4. Average star-formation histories  
6.5. Star formation rates  
6.6. Dust  
6.7. Comparisons with GALEX  

7. CONCLUSIONS