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Fig. 7

image

Configuration of the OGLE-2017-BLG-0604 lens system. Upper right inset: close-up view of the planetary caustic and the source trajectory. Two lower left insets: configurations of the two degenerate solutions obtained from modeling with only the OGLE data, which do not cover the first part of the anomaly at HJD′ ~ 7869.6. These degenerate solutions cannot explain the first part of the anomaly, although they describe the second part of the anomaly as the presented solution almost equally well.

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