The radio properties of z > 3.5 quasars: Are most high-redshift radio-loud active galactic nuclei obscured?

Open Access

Fig. 2.

Distribution of the length of the major axis, r_maj., obtained from a two-dimensional Gaussian fit on the VLASS images of the 29 HzRQs. The dashed vertical line marks the median value of r_maj. of the VLASS sources in the same range of declination, and the two dotted lines mark the observed spread of $\sim 0 \overset{″}{.} 4$ ${\sim}0{{\overset{\prime\prime}{.}}}4$ observed for r_maj..

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