Fig. 5
Median-likelihood estimate of the total dust luminosity plotted against star formation rate for the ULIRGs in our sample (both derived from our SED fitting). The red line shows the Kennicutt (1998) relation for optically-thick starbursts, corrected for Chabrier (2003) IMF (Eq. (6)). The error bars correspond to the 16th–84th percentile range of the likelihood distributions of each parameter.
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