EDP Sciences
Free Access
Issue
A&A
Volume 514, May 2010
Article Number A67
Number of page(s) 51
Section Extragalactic astronomy
DOI https://doi.org/10.1051/0004-6361/200913634
Published online 28 May 2010

Online Material

Appendix A: Long tables and figures.

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.

\begin{figure}
\par\includegraphics[width=15.5cm,clip]{fA1.eps}
\end{figure} Figure A.1:

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: $3\sigma $ upper limit (values marked at the base). In the cases where our fits strongly underpredict the observed data at $850~\mu$m, we adopted $L_{\rm IR}$and $T_{\rm d}$of Chapman et al. (2005).

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\begin{figure}
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\end{figure} Figure A.1:

(continued).

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(continued).

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(continued).

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(continued).

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(continued).

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(continued).

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(continued).

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(continued).

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(continued).

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Table A.4:   Compilation of star formation rate density determinations in $M_\odot~\mbox{yr}^{-1}~\mbox{Mpc}^{-3}$.

Table A.5:   Compilation of stellar mass density determinations in $\log M_\odot~\mbox{Mpc}^{-3}$.

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