1. Introduction

2. Design of the SHINE survey
2.1. The SHINE database
2.2. Target priorities
2.3. Simulations of planet detectability

3. The final SHINE target list

4. The F150 sample

5. Updated stellar properties
5.1. Distance and proper motion
5.2. Radial velocity
5.3. Multiplicity
5.4. Kinematics and moving group membership
5.5. Chromospheric and coronal activity
5.6. Lithium
5.7. Photometric variability and rotation period
5.8. Isochrone fitting
5.9. Adopted ages
5.10. Stellar masses
5.11. Presence of disks

6. Sample properties
6.1. Comparison with GPIES and other surveys

7. Summary and conclusions