Fig. 3.
K2 light curve (represented by red points) of eclipsing binary OGLE-BLG-ECL-234840 derived using MCPM with model light curve (indicated by a blue line) predicted using ground-based data and a three-parameter fit (Eq. (11)). The y-axis units are K2 flux units where the photometric zero point of the magnitude scale corresponds to Kp = 25 mag. Lower panel: residuals of the fit.
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