1. Introduction
2. Sample properties
2.1. Distance and proper motion
2.2. Radial velocities
2.3. Stellar ages
2.4. Stellar masses
3. Observations and data reduction
3.1. Standard SHINE reduction
3.2. Manual detections on non-coronagraphic observations
3.3. Automatic detections on non-coronagraphic observations
3.4. Detection limits
4. Results
4.1. SPHERE astrometry and photometry
4.2. Gaia astrometry and photometry
4.3. Common proper motion confirmation
4.4. Constraints on the binary orbits
4.5. Sensitivity to additional companions
5. Discussion
5.1. Survey completeness and binary frequency
5.2. Mass ratio distribution
5.3. Dynamical masses
5.4. Orbital parameters
5.5. Spin-orbit alignment
6. Conclusions and final remarks