Example of the correction of the PSF effect applied to NGC 3486 in FUV. Left panel: Profile after background subtraction (red), the profile from the Wiener deconvolved image (black), and the profile after applying all the PSF deconvolution procedures (blue). Middle panel: Exponential fit (cyan) to the Wiener deconvolved image after the edge of the galaxy (in this case R_J = 195″). Right panel: Model (Wiener “core” plus exponential outer region) convolved with the extended PSF (yellow). This model is compared to the profile of the galaxy in the original with the background subtracted.