(Sub)stellar companions identified in SPHERE data. We present the derotated and median combined coronagraphic images for the epochs and filters as indicated in the upper right of each panel. The star is located behind the coronagraphic mask at the center of each panel. The companions that were also identified by our Gaia selection algorithm are highlighted by the white arrows. As discussed in Sect. 4.2.4, there is an additional, very close companion to 2MASS J12560830-6926539. With a separation of merely 0′′.2 this stellar companion is not identified by our Gaia selection method. In the lower-left section of each panel, we present the non-coronagraphic flux PSFs of each target. In all frames north points up and east towards the left.