Fig. 13.
TESS light curves of SW CMa (top), V1647 Sgr (middle), and V477 Cyg (bottom). Left: TESS light curves phased with the orbital periods. Phase 0.5 corresponds to the epoch of the periastron passage. Right: zoom of the light curve after cutting out the eclipses. Continuous dark blue line is the fitted Kumar’s model. For comparison, the dashed line shows the fit of Kumar’s model with inclination fixed at the value given in Table A.1.
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