Example light curves illustrating the capabilities and limitations of our correction process. Panel (a) shows the light curve of an eclipsing binary with a significant primary eclipse and a secondary eclipse that only becomes really apparent after the correction was carried out. Panel (b) shows a star where the instrumental systematics completely obscure the intrinsic signal despite their being of comparable amplitude. Panel (c) shows the light curve of a star located at the edge of the superstamp and which suffers from artifacts created by the correction process as a consequence. Each panel includes highlighted regions to show the details of the relevant effects.