Comparison between the main physical quantities derived in K22 and the ones derived in this study when applying HEISENBERG to the same CO and Hα maps, within masks that correspond to the MIRI/21 μm observations, and adopting an updated CO-to-H₂ conversion factor (see Section 3.1). Left: Comparison of the predicted molecular gas masses (upper left panel), H₂ gas surface density (upper-right panel), SFR (bottom left panel), and SFR surface densities (bottom-right panel). Deviations remain moderate between both studies: most of our sample lie on the one-one relation while the few galaxies that deviate from previous measurements remain in good agreement within a factor of 2. Right: Comparison between the cloud lifetimes (t_gas = t_CO) derived in K22 and the ones derived in this study when applying HEISENBERG to the same CO and Hα maps, within masks that correspond to the MIRI/21 μm observations. Both measurements are in agreement within a factor of 1.5.