Investigating the age-velocity relation of NGC 4030. Panel a: AVR of NGC 4030 accounting for all bins displaying luminosity-weighted ages obtained with FADO. Values of the redshift at each τ_⋆,L are provided along the upper horizontal axis. Panel b: Radial profiles of the observed σ_⋆ obtained for the whole map (grey) and for a subset of spaxels that show increasing levels of EW(Hα) (in blue, with lighter shades corresponding to higher EW(Hα) levels). Panel c: Similar to panel a but illustrating the radial distribution of the luminosity-weighted stellar age.