1. Introduction

2. The Data Set
2.1. Correction for absorption for the X-ray luminosity

3. Rest-frame monochromatic fluxes and Spectral Energy Distributions

4. Average SED

5. SED-fitting
5.1. Template libraries

6. Bolometric luminosities and bolometric corrections

7. Robustness of the method

8. Results and discussion
8.3. Host-galaxy properties: M*, SFR, colors and morphologies

9. Summary and Conclusions