Disk around GSC 07396-00759, as seen with SPHERE/IRDIS in polarized light (top-left panel) and total intensity (top-right panel; Sissa et al. 2018) in the H-band. The bottom panels show the best-fit disk model found in this work (bottom left) and found by Sissa et al. (2018) in the same scaling as the according observations. The dash-dotted line is parallel to the disk semimajor axis and crosses the central star.The coronagraphic mask is indicated by the (shaded) circular region in each panel.