Fig. 5.
From: Star formation and dust extinction properties of local galaxies as seen from AKARI and GALEX
Relation between LFUV and LTIR. The diagonal dotted line represents the case if LFUV equals LTIR. Black dots represent the data from Takeuchi et al. (2010). Downward arrows represent galaxies which have UV flux densities below the detection limit of GALEX.