which achieve 5$\sigma$ flux density limits of $\sim$2 mJy [@Frayer:06]. The best fit to the 16$\mu$m, 22[$\mu$m]{} and 24$\mu$m photometry is from a starburst source with strong PAH emission at $z=1.7$. The increase in the 22$\mu$m and 24$\mu$m flux relative to 16$\mu$m is due to the entrance of the 7.7$\mu$m PAH complex into the 22$\mu$m and 24$\mu$m bandpasses. The flux in the 16$\mu$m bandpass is lower since the 6.2$\mu$m PAH feature is much weaker.

Extrapolating the templates that are fit to the mid-infrared photometry also yields an estimate of the far-infrared luminosity for the galaxy. The L$_{\rm IR}$=L(8$-$1000[$\mu$m]{}) luminosity of the source is $\sim$5$\times$10$^{11}$ L$_{\sun}$, which corresponds to a star-formation rate of 80 M$_{\sun}$ yr$^{-1}$. We compare this with optical/UV estimates of star-formation in the following section. Using the radio-FIR correlation in @Yun, we predict the 1.4 GHz to be 12$\mu$Jy and the 8.4 GHz flux density to be 3.7$\mu$Jy while the predicted fluxes at 70[$\mu$m]{} and 850[$\mu$m]{} are shown in Table 1. The deepest 70[$\mu$m]{} and 850[$\mu$m]{} surveys are currently sensitive to 1.5$-$2 mJy. The predicted intensities of JD2 are below these limits implying that confirmation of the derived far-infrared luminosity will have to await deeper observations by [*Herschel*]{} 