Images of sources with different radio morphologies seen in VLA. Contours are drawn using the parameters shown in Table E.1. The first three images correspond to small FRI sources like those selected in Capetti et al. (2017b) (the first was excluded from our sample because of its FIRST morphology). The fourth image corresponds to a WAT source (see Owen & Rudnick 1976) and the last image shows a star-forming galaxy excluded from the sample.