AGN populations in the local Universe: Their alignment with the main sequence, stellar population characteristics, accretion efficiency, and the impact of AGN feedback

Open Access

Fig. 2.

AGN luminosity at 12 μm as estimated by CIGALE versus observed X-ray luminosity in the 2–10 keV band for our sample of local SDSS AGN. Gray circles correspond to LINER+Composite objects, and red circles are Seyfert 2 galaxies. Symbols marked with a horizontal and/or vertical bar show upper limits in the 12 μm and/or X-ray luminosity, respectively. The black, dashed line shows $log (L_{X}^{obs} / L_{12 μ m}^{SGN}) = - 1.6$ $\log(L_{\mathrm{X}}^{\mathrm{obs}} / L_{12\,{\upmu}\mathrm{m}}^{\mathrm{SGN}}) = -1.6$ .

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