Fig. 4
Spots on researched systems. Top: 3D reconstruction of ASAS-04 (left) and ASAS-08 (right) during the primary (φ = 0.02) and secondary eclipse (φ = 0.48). Units are solar radii, scale is the same for both systems; bottom: influence of spots on the ASAS-04 and ASAS-08 light and RV curves. The absolute difference between a spotted and non-spotted case is plotted. Differential RV curves are overplotted on RV residuals, the same as in Fig. 1.
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