Fig. 16
Observed LIR/LUV luminosity ratio vs. LUV for our sample. Solid and dashed gray lines show the limits for LIRGs and ULIRGs respectively, and the pink dotted line the mean relation derived from stacking for z ~ 1.5 UV-selected galaxies by Heinis et al. (2013). On the embedded vertical axis we have the corresponding UV attenuation from Schaerer et al. (2013). The individual objects are ordered from left to right as follows: C0, HLS115, nn4, MACS0451, cB58, h7, and the Eye.
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