Fig. 1.
From: Star formation and dust extinction properties of local galaxies as seen from AKARI and GALEX

LTIR and LFUV distributions of our sample. Dashed and solid histograms represent the distributions of LFUV and LTIR, respectively.
From: Star formation and dust extinction properties of local galaxies as seen from AKARI and GALEX
LTIR and LFUV distributions of our sample. Dashed and solid histograms represent the distributions of LFUV and LTIR, respectively.