Fig. 7
PHOEBE models for two identical G-type stars in a ~14.4-day orbit, for an inclination of 74.6° and 73.8° (red and black continuous lines, respectively). Top: zoom-in around the eclipses. Time is given in hours. Horizontal and vertical dashed lines indicate the transit duration and depth, respectively, for visual inspection. Bottom: complete orbits, highlighting the continuum flux variability.
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