Fig. 9.
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TESS photometry of V889 Aql from the second orbit of Sector 40 (black dots) and its best fit computed with JKTEBOP (red). The top panel shows the photometry phase-folded to the sidereal period, while the bottom panel shows the details of the primary (left) and secondary (right) eclipses. The residuals of the fits are shown in the bottom part of all panels.
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