All Tables

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.
Table 2: Estimates of critical angles, ${\theta }_{\rm cs}$ and ${\theta }_{\rm cf}$ and their errors in equal subsamples binned by $L_{[\rm O~III] }$ . The first line of the table refers to the two sets of binned data, and the second line shows results of three sets of binned data.
Table 3: The significance (Fisher test) of the null hypothesis that the ${\theta }_{\rm cs}$ are equal in two equal subsamples divided by $L_{[\rm O~III] }$ , $L_{\rm {151}}$ and redshift z, respectively. Probabilities are calculated for: (1) the sample which includes 20 WQs grouped with HEGs rather than quasars; (2) the sample consisting only of HEGs and quasars; and (3) the sample which excludes 12 transitional sources with $\log~(L_{151}$ / W Hz^-1 sr ^-1) < 25.3.
Table 4: The values of true critical angles $\theta _{\rm ct}$ and their deviations ( ${\theta }_{\rm cs}$ ) simulated for different half cone angles $\delta _{\rm max}$ within which the angles between the axes of the torus and the jet are distributed.