All Figures

$\begin{figure} \par\includegraphics[width=13.2cm,clip]{4664f01.eps} \end{figure}$ Figure 1: Results of decomposition. As an example, we only show 4 representative Seyfert 2s with the smallest to the largest $\chi ^2$ (NGC 3035, NGC 5252, NGC 5643 and NGC 7582, from top to bottom). For each source, we show the original image ( left), the model ( middle) fitted by GALFIT, and the residual image ( right).
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.1cm,clip]{4664f02.eps} \end{figure}$ Figure 2: The AGN $K_{\rm S}$ -band absolute magnitude versus [O III] $\lambda$ 5007 luminosity. Red open-square symbols correspond to Seyfert 2s with direct evidence of hidden broad-line regions (HBLR) from spectropolarimetric observations. The dashed line shows a ordinary least square (OLS) bisector fit to the data of slope $-0.715\pm 0.051$ . The Spearman rank-order correlation coefficient ( $R_{\rm S}$ ) is -0.52 and the null probability is 0.0004.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{4664f03.eps} \end{figure}$ Figure 3: The AGN $K_{\rm S}$ -band absolute magnitude versus 2-10 keV hard X-ray luminosity. The dashed line shows an OLS bisector fit to the data of slope $-0.406\pm 0.124$ . The Spearman rank-order correlation coefficient ( $R_{\rm S}$ ) is -0.54 and the null probability is 0.0008. Symbols have the same meaning as in Fig. 2.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{4664f04.eps} \end{figure}$ Figure 4: The bulge's $K_{\rm S}$ -band absolute magnitude versus the black hole mass. The dashed line shows an OLS bisector fit to the data of slope $1.199\pm 0.080$ . The Spearman rank-order correlation coefficient ( $R_{\rm S}$ ) is 0.59 and the null probability $4.6 \times 10^{-6}$ . Symbols have the same meaning as in Fig. 2.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=13.2cm,clip]{4664f01.eps} \end{figure}$	Figure 1: Results of decomposition. As an example, we only show 4 representative Seyfert 2s with the smallest to the largest $\chi ^2$ (NGC 3035, NGC 5252, NGC 5643 and NGC 7582, from top to bottom). For each source, we show the original image ( left), the model ( middle) fitted by GALFIT, and the residual image ( right).
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{4664f03.eps} \end{figure}$	Figure 3: The AGN $K_{\rm S}$ -band absolute magnitude versus 2-10 keV hard X-ray luminosity. The dashed line shows an OLS bisector fit to the data of slope $-0.406\pm 0.124$ . The Spearman rank-order correlation coefficient ( $R_{\rm S}$ ) is -0.54 and the null probability is 0.0008. Symbols have the same meaning as in Fig. 2.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{4664f04.eps} \end{figure}$	Figure 4: The bulge's $K_{\rm S}$ -band absolute magnitude versus the black hole mass. The dashed line shows an OLS bisector fit to the data of slope $1.199\pm 0.080$ . The Spearman rank-order correlation coefficient ( $R_{\rm S}$ ) is 0.59 and the null probability $4.6 \times 10^{-6}$ . Symbols have the same meaning as in Fig. 2.
Open with DEXTER