Notes. The values listed here are for the galaxies within the full stellar mass range listed in Table 1. Visual classifications are only available for galaxies from the FDS (cluster) and ELVES (satellite) samples. The rest of the sample has been categorised using the equivalent widths of the Hα line as a proxy for star forming or quenched systems. We used this categorisation as late- or early-type, respectively (see text for details).