Figure 4. Fits to rest-frame photometry for individual GDDS galaxies. A hot greybody + PAH model (the dashed
blue line) is seen to do an excellent job of boosting the flux from starlight at rest wavelengths around 3 μm
in order to fit the data. Mentuch et al. (2009) shows how such a model is consistent with emission from a hot
circumstellar torus around massive young stars.
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GeminiFocus
June2012