Table 1: The Kolmogorov-Smirnov test is used to estimate the significance level of the hypothesis that the [O III] emission-line luminosity (and radio luminosity) distributions of HEGs and quasars (QSOs), HEGs and WQs, and, QSOs and WQs are drawn from the same parent distribution.

\begin{displaymath}\begin{tabular}{cccc} \hline \hline \noalign{\smallskip } ... ...G-WQ & 79.47 \\ \noalign{\smallskip } \hline \end{tabular} \end{displaymath}


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Article Contents
1 Introduction
2 Equations for the opening angle of the torus
3 The sample and selection criteria
4 Relations for the torus opening angle
5 Discussion and conclusions
Appendix: Equation for estimating the critical viewing angle
References
List of tables
List of figures