Upper panels: white-light images obtained after co-adding the data using classical ADI (left panel) and with the LOCI algorithm (right panel) for the first and second nights respectively. The planet is visible near [0.2′′, −0.3′′], but is barely recovered in the second night, and not distinguishable from speckle noise in the first night. Lower panels: cross-correlation maps using the preferred BT-Settl model (T_eff =1700 K and log (g) = 3.5). The colour scales linearly from black to white between −0.1 and +0.5 (left panel) and −0.05 to +0.25 (right panel).