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Fig.10

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Same as Fig. 9, but on a wider flux density scale and with the addition of ACT (Marriage et al. 2011) and SPT (Vieira et al. 2010) data shown as squares at 143 and 217 GHz, and SCUBA and LABOCA data shown as stars at 353GHz (Borys et al. 2003; Coppin et al. 2006; Scott et al. 2006; Beelen et al. 2008; Weiss et al. 2009). Notice that we added the model of Bethermin et al. (2011) at 500  μm (dash-dot) to comply with the Herschel data taken at that wavelength (and not at 545 GHz).

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