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Fig. 4

image

Best-fits of the ALMA-detected SMG. The black symbols show the measured fluxes, the grey symbols those estimated through assumptions in the Herschel bands (see text). The upside-down grey triangle shows the total 24 μm flux of the blended system. The blue curve shows the best fit of the optical-to-NIR photometry with the Bruzual & Charlot (2003, BC03) library; the brownish curve is the best fit of all available bands with the SMG templates of Michałowski et al. (2010b); the red and orange curves are the fit of the ALMA flux to the average SMG templates of Michałowski et al. (2010b) and Pope et al. (2008), respectively; the light green curve represents the best fit of the Draine & Li (2007) library to the Herschel and ALMA bands; finally, the dark green curve is the fit with a modified blackbody with emissivity index β = 2 to the 160 μm-to-ALMA bands. See text for further details.

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