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Fig. 2.

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Folded and fitted TESS sector 26, 40, and 53 light curves of the wide binary companion V815 Her B. Cleaned observations are marked with blue dots, the original orbital solutions without assuming surface inhomogeneities are drawn with gray lines, while the models drawn with red lines fit also the light curve variations arising from stellar spots. The residuals of both fits are plotted on the bottom parts of all panels. We note that the eclipses in sectors 40 and 53 (middle and bottom panels) are shifted from phases 0.0 and 0.5, indicating timing variations, which are discussed in detail in the text.

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