Fig. 6.
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Position angle of the major axis of the [O III]λ5007 and the radio emission for the galaxies in the Jarvis et al. (2019) sample and our targets. Sources located within the gray dashed lines are considered aligned (see Section 6.1). XID-36 does not show any extended structures, and the radio emission is poorly resolved; therefore, we do not have a reliable radio PA for this object.
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