Comparison between the physical properties of LVL galaxies, derived using the CIGALE parameter space used in this work (introduced in Nersesian et al. 2019) and those of Dale et al. (2023). Stellar mass, dust mass and SFR are shown in the left, middle and right panel, respectively. A black-dashed line indicates the one-to-one relation. In the middle panel, a dark-red dash-dotted line shows the y= x - 0.42 relation; for 50 objects, Dale et al. (2023) only provide upper limits for M_dust, which are indicated with a different symbol.