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Fig. 3


Spectral energy distribution from the IR (Bouchet et al. 2006; Seok et al. 2008; Dwek et al. 2010; Matsuura et al. 2011) to the radio (Manchester et al. 2005; Potter et al. 2009; Zanardo et al. 2010), including our first measurements at sub-mm (APEX) and mm (ATCA) wavelengths. Overplotted are modified blackbodies to represent two dust components, two steep radio powerlaws to represent synchrotron radiation, and two shallow powerlaws to represent free-free radiation. Cyan and magenta curves represent the sum of all emission for the 2004–5 and 2007–10 period, respectively, with residuals plotted underneath.

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