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Published online by Cambridge University Press: 01 December 2006
Properties related to dust attenuation and star formation of an UV selected sample of intermediate redshift galaxies are presented in this work. We find hints of a decrease of the LIR/LFUV ratio with increasing redshift at low values of the total luminosity. Downsizing is observed at all redshifts, and the SSFR is found to increase with increasing redshift at all stellar masses.