Table A.1: Photometry detections of SMGs.
Table A.2: Photometry upper limits of SMGs.
Table A.3: Properties of SMGs derived from the SED modeling.
Spectral energy distributions (SEDs) of SMGs. Solid lines: the best GRASIL fits. Dashed lines: SEDs of GRB hosts (Michaowski et al. 2008) shown for comparison. Squares: detections with errors, in most cases, smaller than the size of the symbols. Arrows: upper limit (values marked at the base). In the cases where our fits strongly underpredict the observed data at m, we adopted and of Chapman et al. (2005).
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Table A.4: Compilation of star formation rate density determinations in .
Table A.5: Compilation of stellar mass density determinations in .