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We built a 8um selected sample of galaxies in the NEP-AKARI field by defining4 redshift bins with the four AKARI bands at 11, 15, 18 and 24 microns(0.15<z<0.49, 0.75<z<1.34, 1.34<z<1.7 and 1.7<z<2.05) . Our sample contains4079 sources, 599 are securely detected with Herschel/PACS. Also addingultraviolet (UV) data from GALEX, we fit the spectral energy distributionsusing the physically motivated code CIGALE to extract the star formation rate,stellar mass, dust attenuation and the AGN contribution to the total infraredluminosity (L_{IR}). We discuss the impact of the adopted attenuation curve andthat of the wavelength coverage to estimate these physical parameters. We focuson galaxies with a luminosity close the characteristic L_{IR}^* in thedifferent redshift bins to study the evolution with redshift of the dustattenuation in these galaxies.

NEP-AKARI: Evolution with redshift of dust attenuation in 8 micron selected galaxies