With its last observation taken in September 2021, the SpHere INfrared survey for Exoplanets (SHINE) is ready to unveil its final performances and results. Using 200 nights of GTO time, the SHINE survey aimed at, among other objectives, discovering and characterize new exoplanets or brown dwarfs, studying planetary architectures and the frequency of giant planets beyond 10 au. Including 400 stars and more than 650 observations, it is, alongside GPIES, the largest survey ever conducted on current high contrast imager. Completely re-analyzed with a state-of-the-art algorithm named PACO, with improved performances up to 1 magnitude compared to what was used in the first half of the survey, we will dive into the observations and the reduction process with an emphasis on point sources classification. Finally, I will present the final performances in term of contrast for the overall sample and some take away messages for future surveys.