Fig. 1
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Light curves of the microlensing event OGLE-2015-BLG-1609 with three microlensing model topologies for positive values of the impact parameter, u0. The difference between the topologies is visible only during the planetary anomaly (HJD ~ 2457270; see Fig. 2). The photometry comes from the OGLE, MOA, RoboNet, and MiNDSTEp projects.
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