Illustration of the deblending capability of our algorithm for pairs of point sources. The upper panels show the photometric accuracy as a function of contrast between the objects and as a function of separation. The astrometric precision is given in the lower panels in units of deconvolved pixels. The vertical red dashed line indicates the FWHM of the PSF in the simulation (7.5 pixels). The horizontal black dashed line indicates a 0.02 pixel precision for reference. The color code represents the S/N of the objects as defined in Eq. (23).