Fig. 2.
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Spectral energy distribution of the main lens galaxy of SDSS J0100+1818. The observed flux densities from NOT (red triangles), Pan-STARRS (red circles), and HST (red square) are used to fit the SED with the CIGALE software. Error bars are smaller than the symbols. The best-fit stellar continuum template (blue curve) corresponds to the model fluxes plotted in orange and is used to infer the total stellar mass value of the deflector. The bottom panel shows the relative residuals of the fit.
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