Fig. 2
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Microlensing light curves of KMT-2017-BLG-0673 and KMT-2019-BLG-0414. The curve drawn over the data points of each light curve is a 1L1S model, and the box indicates the region of the anomaly. The enlarged views of the anomaly regions are shown in Fig. 3 for KMT-2017-BLG-0673 and in Fig. 4 for KMT-2019-BLG-0414. Colors of data points are set to match those of the telescopes marked in the legend.
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