Postage stamps showing the lens galaxy fitting with GALFIT for the newly discovered HAH grade A candidates. Three lens candidates are presented per line; each HAH lens is indicated by the sequence part of the name. Each postage stamp is composed of (1) the original image used for the fit using the HST instruments and filters indicated in Tables A.1 and A.2, (2) the fitted model using chi-square minimisation in GALFIT, and (3) the residuals obtained by subtracting the fitted model from the original image. The arcs and background galaxies were masked using SExtractor during the fitting process, and thus only the light of the lens was fitted. The postage stamps show the default orientation of the HST images, which can be different from that shown in Fig. 2.