Relationships between global and beam quantities, namely star formation efficiency, SFE, left column, and molecular gas fraction f_mol, right column, colour-coded by the distance from the SFMS (ΔSFMS, top row), morphology (middle row), and the different samples included in the database (bottom row). In the panels, the black full line shows the 1:1 locus, while grey dotted lines are separated by 1 dex. The black dashed lines in the left column indicate a τ_dep = 2 Gyr. In the top row, the yellow pentagons show the positions of the wAGN-hosts in the sample, while the yellow stars show the positions of sAGN-hosts. In the middle row, dark blue dots show the locations of the SAB/SB galaxies. In the panels, the transparent diamonds are used to indicate that a given measurement is obtained with a CO upper limit. While f_mol does not appear to vary across the galaxy discs, the SFE in the centre of the retired early-type galaxies in particular is ~1 dex lower compared to the SFE across the entire galaxies.