Online material
Table 1
SED of Type-2 QSOs.
Table 2
Morphological parameters of Type-2 QSO hosts at z ≤ 1.2.
Appendix A: SED fits
SED decomposition for the sample of Type-2 QSOs. Black circles are the observed photometry in the rest-frame. Purple and blue lines correspond respectively to the galaxy and AGN template found as the best fit solution, while the black line shows their sum. The triangle is the predicted AGN emission at 12.3 μm based on the Gandhi et al. (2009) correlation. We tried to anchor the AGN template to this value allowing an uncertainty egual to the dispersion observed by Gandhi et al. (2009) in their correlation.
© ESO, 2011