Left panel: β vs. IRX plot for our three candidates detected in GOODS-Herschel. The Meurer et al. (1999) data and relation have been corrected with the 1.75 factor as quoted by Reddy et al. (2010), to convert from L_FIR to the total L_IR. Also shown are the more recent Takeuchi et al. (2012) and Buat et al. (2012)β-IRX relations, derived for local galaxies and z ~ 1−2 sources, respectively. Right panel: IRX vs. bolometric luminosity for the same candidates, compared to the sample of BzK selected galaxies from Daddi et al. (2007) and the empirical relation for BM/BX-selected galaxies found by Reddy et al. (2006).