Cosmic evolution of submillimeter galaxies and their contribution to stellar mass assembly

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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$\begin{figure} \par\includegraphics[width=15.5cm,clip]{fA2.eps} \end{figure}$	Figure A.1: (continued).
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$\begin{figure} \par\includegraphics[width=15.5cm,clip]{fA3.eps} \end{figure}$	Figure A.1: (continued).
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$\begin{figure} \par\includegraphics[width=15.5cm,clip]{fA4.eps} \end{figure}$	Figure A.1: (continued).
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$\begin{figure} \par\includegraphics[width=15.5cm,clip]{fA5.eps} \end{figure}$	Figure A.1: (continued).
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$\begin{figure} \par\includegraphics[width=15.5cm,clip]{fA6.eps} \end{figure}$	Figure A.1: (continued).
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$\begin{figure} \par\includegraphics[width=15.5cm,clip]{fA7.eps} \end{figure}$	Figure A.1: (continued).
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$\begin{figure} \par\includegraphics[width=15.5cm,clip]{fA8.eps} \end{figure}$	Figure A.1: (continued).
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$\begin{figure} \par\includegraphics[width=15.5cm,clip]{fA9.eps} \end{figure}$	Figure A.1: (continued).
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$\begin{figure} \par\includegraphics[width=15.5cm,clip]{fA10.eps} \end{figure}$	Figure A.1: (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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