Fig. 10
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Light curve and model for KMT-2018-BLG-2164. The anomaly is a dip centered at 8290.8. Similar to KMT-2018-BLG-2718, this anomaly is subject to the Han & Gaudi (2008) planet binary degeneracy (see insets), but contrary to that case, the planetary interpretation is not decisively favored (see Table 10). Therefore, the lens companion cannot be claimed as a planet.
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