Citations:bolometrically


 * 2010 Naveen A. Reddy et al, "Dust Obscuration and Metallicity at High Redshift: New Inferences from UV, H-alpha, and 8 Micron Observations of z~2 Star-Forming Galaxies" arXiv
 * Our results provide the first direct evidence, independent of the UV slope, for a correlation between UV and bolometric luminosity at high redshift, in the sense that UV-faint galaxies are also on average less infrared and less bolometrically-luminous than their UV-bright counterparts.