SED fitting model and photometric data. In the upper panel, we show the fitted SED model spectrum from X-CIGALE with a black curve. In addition, dust and unattenuated stellar and AGN emissions are shown in red, blue dotted, and yellow curves, respectively. The input observed photometry flux densities are marked in dark magenta boxes and olive triangles (upper limits). The X-ray data are not shown as they do not constrain the stellar component. The green vertical dashed line is the position of rest frame 1.6 μm from which the unattenuated stellar flux is adopted for M_stellar estimation. In the lower panel, we present the relative residuals, , where S_ν,obs and S_ν,mod are the observed and model flux densities, respectively.