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Fig. 14


Resulting fluxes from the 1BB model fit in the high temperature epoch 5, plotted over wavelength. Overplotted are our derived NIR and MIR fluxes (zYJHK and W1, W2, W3). The 1BB model roughly matches the MIR point source fluxes, given by Burtscher et al. (2009). Since the model was fit to our zYJHK data alone (also see Sect. 5.2), these are marked with green circles, while the other data are represented by triangles.

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