Light curve of KMT-2016-BLG-2364. The dotted and solid curves superposed on the data points are the lL1S and 2L1S models, respectively. The lensing parameters of the 2L1S model are presented in Table 2. Upper panels: enlarged views of the regions around HJD′ ~ 7601 (left panel) and ~7607 (right panel) when the planet-induced anomalies occur. The lens system configuration of the 2L1S solution is presented in Fig. 2.