Notes. Columns indicate: (2) Cazzoli et al. (2018), (3) Hermosa Muñoz et al. (2020), (4) HM22, and (5) this work (C18, HM20, HM22 and This work, respectively). “Inflow” and “Outflow” indicate candidates of hosting an inflow or an outflow, “Rotation” indicates those for which the kinematical components were consistent with being produced by rotational motions, “Candidate” indicates those candidates for non-rotational motions. “Bubble” refers to bubble-like, filamentary emission; “Core-halo” to compact emission in the circumnuclear region; and “Dusty” when dust lanes covered the central parts of the galaxy. A complete definition of the latter three categories can be found in HM22.