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AKARI/Infrared Camera (IRC) Point Source Catalog provides a large amount offlux data at {\it S9W} ($9\ {\rm \mu m}$) and {\it L18W} ($18\ {\rm \mu m}$)bands. With the goal of constructing Star-Formation Rate(SFR) calculationsusing IRC data, we analyzed an IR selectedGALEX-SDSS-2MASS-AKARI(IRC/Far-Infrared Surveyor) sample of 153 nearbygalaxies. The far-infrared fluxes were obtained from AKARI diffuse maps tocorrect the underestimation for extended sources raised by the point-spreadfunction photometry. SFRs of these galaxies were derived by the spectral energydistribution fitting program CIGALE. In spite of complicated features containedin these bands, both the {\it S9W} and {\it L18W} emission correlate with theSFR of galaxies. The SFR calibrations using {\it S9W} and {\it L18W} arepresented for the first time. These calibrations agree well with previous worksbased on Spitzer data within the scatters, and should be applicable todust-rich galaxies.

AKARI/IRC Broadband Mid-infrared data as an indicator of Star Formation Rate