Astronomy & Astrophysics

All Figures

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{DistriNhSy2PBL.eps}\end{figure}$ Figure 1: Hydrogen column density distributions of Sy 2 with polarized broad lines (upper panel) and without PBL (lower panel).
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{DistriLumPBL.eps}\end{figure}$ Figure 2: Luminosity distributions of Sy 2 with polarized broad lines (upper panel) and without PBL (lower panel).
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{DefPBLNewNPBL.ps}\end{figure}$ Figure 3: Average spectra of Seyfert 2 galaxies with (black) and without (light red) polarized broad lines.
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In the text

$\begin{figure} \par\includegraphics[width=13cm,clip]{NEWRatioPBL.eps}\end{figure}$ Figure 4: Left: average spectra of Sy 1, PBLs and NPBLs galaxies (upper panel) and the normalized ratio of Spectral Energy Distributions of the pair PBLs/NPBLs (lower panel). Right: ratios of SEDs of the pairs: PBLs/Sy 1 and NPBLs/Sy 1 galaxies.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{RebinPBLNPBL_7.eps}\end{figure}$ Figure 5: Normalized ratio of rebinned spectra of the pair PBLs/NPBLs.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{RatioModels.eps}\end{figure}$ Figure 6: Ratios of models corresponding to the best fits. The models are respectively a cutoff power law for PBLs ( $\Gamma$ $_{\textrm{\tiny{PBL}}}^{\textrm{\tiny{CPL}}}=$ 1.38, $E_{\rm c}=$ 83.6 keV) and Sy 1 galaxies ( $\Gamma$ $_{\textrm{\tiny{Sy1}}}^{\textrm{\tiny{CPL}}}=$ 1.49, $E_{\rm c}=$ 70 keV), and a simple power law for NPBLs ( $\Gamma$ $_{\textrm{\tiny{NPBL}}}^{\textrm{\tiny{PL}}}=$ 1.99).
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.8cm,clip]{DefAverPBL_po.ps}\end{figure}$ Figure A.1: Average spectrum of Seyfert 2 galaxies with polarized broad lines fitted by a power law model and residuals.

In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.8cm,clip]{DefAverPBL_cpl.ps}\end{figure}$ Figure A.2: Average spectrum of Seyfert 2 galaxies with polarized broad lines fitted by a cutoff power law model and residuals.

In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.8cm,clip]{DefAverPBL_pex.ps}\end{figure}$ Figure A.3: Average spectrum of Seyfert 2 galaxies with polarized broad lines fitted by the PEXRAV model (cos $\theta$ = 0.45) and residuals.

In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.8cm,clip]{DefNPBLaver_po.ps}\end{figure}$ Figure A.4: Average spectrum of Seyfert 2 galaxies without polarized broad lines fitted by a power law model and residuals.

In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.8cm,clip]{DefNPBLaver_cpl.ps}\end{figure}$ Figure A.5: Average spectrum of Seyfert 2 galaxies without polarized broad lines fitted by a cutoff power law model and residuals.

In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.8cm,clip]{DefNPBLaver_pex.ps}\end{figure}$ Figure A.6: Average spectrum of Seyfert 2 galaxies without polarized broad lines fitted by the PEXRAV model (cos $\theta$ = 0.45) and residuals.

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{DistriNhSy2PBL.eps}\end{figure}$	Figure 1: Hydrogen column density distributions of Sy 2 with polarized broad lines (upper panel) and without PBL (lower panel).
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{DistriLumPBL.eps}\end{figure}$	Figure 2: Luminosity distributions of Sy 2 with polarized broad lines (upper panel) and without PBL (lower panel).
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$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{DefPBLNewNPBL.ps}\end{figure}$	Figure 3: Average spectra of Seyfert 2 galaxies with (black) and without (light red) polarized broad lines.
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$\begin{figure} \par\includegraphics[width=13cm,clip]{NEWRatioPBL.eps}\end{figure}$	Figure 4: Left: average spectra of Sy 1, PBLs and NPBLs galaxies (upper panel) and the normalized ratio of Spectral Energy Distributions of the pair PBLs/NPBLs (lower panel). Right: ratios of SEDs of the pairs: PBLs/Sy 1 and NPBLs/Sy 1 galaxies.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{RebinPBLNPBL_7.eps}\end{figure}$	Figure 5: Normalized ratio of rebinned spectra of the pair PBLs/NPBLs.
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