Intensity image in the J band of the field around WRAY 15-1880 from the 2016 SPHERE observation after application of the ASDI PCA data analysis technique (Mesa et al. 2015). Top: Image obtained after subtraction of the first 10 modes. Middle: Image obtained after subtraction of the first 25 modes. Bottom: Image obtained after subtraction of the first 50 modes. North is up, east is to the left. The regions within 13 pixels (~97 mas, i.e., behind the coronagraphic mask) and beyond 115 pixels (858 mas, i.e., beyond the IFS field of view) from the star were masked. In all panels a yellow arrow indicates the candidate planet.