ABSTRACT:
Dust obscuration has a profound influence on our view of distant galaxies, and can shed light on star formation processes at high redshift. I will review recent efforts to examine the dust attenuation and bolometric star formation rates of typical (L*) star-forming galaxies at redshifts z~2, incorporating UV, H-alpha, Spitzer, and Herschel observations. I will discuss the trend of dust obscuration with bolometric luminosity and redshift, and the implications for the metallicity evolution of galaxies. I will conclude by showing how these multi-wavelengt