1. Introduction and context
2. The SHINE survey
2.1. Observations setup
2.2. Observations Optimized planning: SPOT
2.3. Observing conditions and Data quality
3. Data Reduction and Analysis
3.1. SPHERE Calibration
3.2. SPHERE Data Center preprocessing
3.3. ADI and ASDI post processing
3.4. Astrometric and Photometric extraction for point sources
4. High contrast Performances
4.1. Contrast curves
4.2. Mass detection limits
5. Exoplanet, Candidate Companion Detections
5.1. Brown dwarfs and exoplanets
5.2. Colours and spectra of detected substellar companions
5.3. Ranking and identification of SHINE candidates
6. Disks detected in SHINE
7. Conclusions and prospects
```