Example SED fit for a [Ne V]-selected AGN of the current sample. The black points with purple error bars are the photometric data, the dark gray line is the best-fit SED, composed of the galactic emission (blue line) and the AGN component (red line). The light grey line is the host galaxy dust emission, the continuous (dashed) green line refers to the dust-obscured (intrinsic) stellar emission. The fitting provides a stellar mass of log(M_*/M_⊙)=10.64 ± 0.05, a SFR of 51 ± 10 M_⊙ yr⁻¹, and an AGN bolometric luminosity of $log(L_{\mathrm{bol}}^{\mathrm{sed}}/{\mathrm{erg}\mathrm{s}}^{-1})=45.6_{-0.1}^{+0.3}$. The bottom panel shows the residuals, where χ = (observation–model)/error.