Poster title: Monitoring of planet variability with SPHERE-IRDIS

Poster abstract: We developed a method to derive the higher photometric precision on close-
in planets, by monitoring the speckle background below them, on SPHERE-IRDIS observations. 
Using this method, we lowered the RMS of the temporal flux on Beta Pictoris b by 2% in K12 
and H23 bands, reaching a 2.5% RMS at best.