Photometric light curves inferred from dT estimates (red circles, left panels) with ZDI fits (green curves), and brightness maps (right panels) reconstructed simultaneously with the magnetic maps of Figs. 2 and 3, for both AU Mic (top row) and EV Lac (bottom row), in the case of Stokes IVQU reconstructions. Very similar results are obtained in Stokes IV reconstructions. The brightness maps are shown as in Figs. 2 and 3, with yellow and blue depicting regions darker and brighter than the quiet photosphere, respectively.