Overview of the Euclid’s ePSFs modelled in our analysis. The top row shows a 3D representation of our ePSFs for the VIS quadrant 1-1.E and for the NISP detector DET11 in each of the three NISP filters. At the top of each panel, we provide the percentage of flux of the star within the centremost pixel, and the full width at half maximum (FWHM) in pixel and in arcsec. The bottom row contains the 2D view of the ePSFs. The scale is logarithmic and the same in all these four panels.