at 3.6, 4.5, 5.8 and 8.0[$\mu$m]{} respectively. The second source, located at 3:32:38.81,-27:48:39.79, is at $z\sim3.1$ with a contribution that is about 0.6 mag fainter at each of the four passbands. We subtracted the contribution of both these sources from the photometry of JD2.

To summarize, the corrected limits for JD2 in the ACS bands are about 0.8 mag brighter due to the larger aperture, the photometry in the NICMOS $J_{110}$ and $H_{160}$ bands is brighter by $\sim10-20$% due to the non-linearity correction and the photometry in the IRAC bands is about 10% fainter on average than those adopted in @Mobasher. The net effect is to reduce the amplitude of the apparent near-infrared to IRAC “break" slightly. The optical/near-infrared photometry of JD2 after these corrections have been applied is shown in Table 2 and which we fit for in Section 3.3. For the sake of completeness, we also investigate redshift constrained fits to the @Dunlop and @Mobasher optical/near-infrared photometry.

In addition, we attempted to fit elliptical isophotes to the galaxy to the SE and subtracted it out from the image. This process left significant residuals due to the asymmetric nature of the [[*Spitzer*]{}]{}/IRAC point spread function. The aperture corrected point 