Same as Figure 2 but for two representative examples of badly fitted SEDs of WDMS candidate binaries. Index number as per the online catalog at the CDS, Gaia DR3 source ID, the values of A_V, ${\chi }_{\mathrm{r}\mathrm{e}\mathrm{d}}^2$, and Vgf_b are mentioned at the top. In the case of source 415 (left), the model spectra are unable to fit the observed flux for majority of data points despite their residual flux ≤50% and Vgf_b value < 15. For source 416 (right), though the model spectra nicely fit the observed fluxes in the UV and optical region but only a couple of observed data points are fitted with MS spectrum due to lack of data points in the NIR regions, hence the fit is not reliable.