Newly detected CCs around transiting exoplanet host stars from the SPHERE/IRDIS data. An unsharp mask was applied to highlight point sources. The origin of the axes is located at the position of the host star. The images are displayed using a logarithmic scale with arbitrary offsets and stretches to highlight the CCs. In all images north points up and east towards the left. The lower left corner of each image shows the reduced non-coronagraphic flux image with the same spatial scale and field orientation.