| Issue |
A&A
Volume 539, March 2012
|
|
|---|---|---|
| Article Number | A48 | |
| Number of page(s) | 41 | |
| Section | Extragalactic astronomy | |
| DOI | https://doi.org/10.1051/0004-6361/201117562 | |
| Published online | 23 February 2012 | |
Online material
Main properties of the sample of 195 Type 1 AGN analysed in this work.
Appendix A
We present here the optical-UV-X-ray SEDs obtained applying the correction discussed in Sect. 3.2, for all the 195 sources analysed in this paper. The filled blue squares represent the fluxes in the GALEX NUV/FUV bands, while the empty squares represent the optical data. The upper limits on the NUV/FUV fluxes are represented as downward arrays. The fit has been done using the model quoted in Sect. 3.4 (blue curve). We also show the slope of the best-fit model in the rest-frame energy range 1–10 keV (magenta curve) obtained from the X-ray spectral analysis (for further details see Corral et al. 2011). The dashed magenta lines represent the errors on the best-fit model of the X-ray data, given by the errors on the spectral index Γ.
© ESO, 2012
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