Fig. 3.
Comparison between the results of the local SED fitting and those of Hanaoka et al. (2019). Each panel shows the comparison of (a) PAH luminosity, (b) hot and warm dust luminosity, (c) cold dust luminosity, and (d) total IR luminosity, respectively. The red lines in each panel correspond to $y=x$. (Color online)

Comparison between the results of the local SED fitting and those of Hanaoka et al. (2019). Each panel shows the comparison of (a) PAH luminosity, (b) hot and warm dust luminosity, (c) cold dust luminosity, and (d) total IR luminosity, respectively. The red lines in each panel correspond to |$y=x$|⁠. (Color online)

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