Left: observed photometry and SED model of AGEL1323 (top) and AGEL0014 (bottom) assuming delayed-τ SFH derived by BAGPIPES (Carnall et al. 2018, 2019). The observed and model photometry are shown by the navy and orange dots, respectively. For AGEL1323, the photometric data are from the DECaLS grz band, HSC ri band, MOSFIRE-YK _s , and HST/WFC3-F140W. For AGEL0014, the photometry is from HSC grizy band and MOSFIRE-JK _s . The orange regions show the 1σ confidence interval of model spectra (light orange) and model photometry (dark orange). Right: posterior distributions and covariances of the lensed stellar mass and the mass-weighted stellar age averaged over the SFH determined from BAGPIPES for AGEL1323 (top) and AGEL0014 (bottom). The contours represent the 1σ, 2σ, and 3σ level.