Top: raw coronagraphic image of ϵ Eri from the observations presented in J. Llop-Sayson et al. (2025). The solid and dotted white contours mark the 1σ and 2σ posterior predictions for ϵ Eri b’s position, respectively. The expected position overlaps with one of the bright PSF lobes, which created strong residuals after PSF subtraction (see Figure 3 in J. Llop-Sayson et al. 2025). Bottom: same as the top panel for the observations presented in this work. The expected position of ϵ Eri b does not overlap with the bright PSF lobes.