TESS light curve of AU Mic. The PDCSAP flux used in the analysis is shown as blue dots. The data considered as flares or transits are shown as red dots. The black and grey lines represent the stellar activity models for the stellar rotation and for the flares, respectively. The flare model was vertical shifted for a better visualisation. The vertical orange and purple bands indicate the timing of the planetary transits for AU Mic b and c, respectively.