Upperleft panel: median over time of the wavelength-collapsed images of HD 169142 obtained with an ADI PCA algorithm, one mode per wavelength. Upper right panel: image obtained by averaging the S/N maps for the individual epochs for IFS. The individual S/N maps are obtained from the ASDI PCA algorithm using 50 components and making a median of the wavelength (see Mesa et al. 2015), and they were rotated for Keplerian motion to the last image before making the median. Lower panel: coincidence image obtained from the same data set. In all panels, the solid line at the bottom of each panel represents 1 arcsec, and a white cross shows the position of the star. N is up and E to the left.