Figure 1. Light curve of OGLE-2018-BLG-0567. The black solid curve on the data is the best-fit 2L1S solution. The upper panel shows the enlarged view of the planet-induced anomaly centered on ¢ ~HJD 8270. The second and fourth panels show the residuals from the solution. The lensing parameters of the solution are listed in Table 1 and the caustic geometry is shown in Figure 3. Note that we use the V-band data only for the source color measurement.
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