Fig. 4.

Representation of the spot configuration of NSVS 10653195 in the (v, w) plane at four phases: from top to bottom, at the primary eclipse (phase 0.0), at the first quadrature (phase 0.25), at the secondary eclipse (phase 0.5), and at the second quadrature (phase 0.75). Both axes have units of relative radius and the images are displaced −0.60 from the previous one. The star in front is orbiting towards the right side and the primary star is the one with two spots.
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