EDP Sciences
Free Access
Issue
A&A
Volume 500, Number 2, June III 2009
Page(s) 705 - 723
Section Extragalactic astronomy
DOI https://doi.org/10.1051/0004-6361/200810630
Published online 19 March 2009

Online Material

 \begin{figure}
\par\includegraphics[width=14cm,clip]{0603fg16.eps}
\end{figure} Figure 13:

Spectral Energy Distribution best-fit models for the MIPS-u sample in units of AB magnitude. The red diamonds represent the observed magnitudes from the photometric data. Non-detections are represented by upper limits. See also Table 3.

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\par\includegraphics[width=14cm,clip]{0603fg17.eps}
\end{figure} Figure 13:

continued.

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\par\includegraphics[width=14cm,clip]{0603fg18.eps}
\end{figure} Figure 13:

continued.

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\par\includegraphics[width=14cm,clip]{0603fg19.eps}
\end{figure} Figure 13:

continued.

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 \begin{figure}
\par\includegraphics[width=14cm,clip]{0603fg20.eps}
\end{figure} Figure 14:

Spectral Energy Distributions of MIPS-d galaxies of our final high-z sample (on the left panels), and the correspondent $\chi ^2_{\nu }$ distributions as a function of redshift ( right panels) in $90\%$ confidence intervals. For each candidate the most probable redshifts (first and second redshift solutions: $z_{\rm phot}$ and  $z_{\rm phot2}$) and the $\chi ^2_{\nu }$ values with the respective probability are also labeled. See also Table 4.

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\par\includegraphics[width=14cm,clip]{0603fg21.eps}
\end{figure} Figure 14:

continued.

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continued.

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 \begin{figure}
\par\includegraphics[width=17.5cm,clip]{0603fg26.eps}
\end{figure} Figure 15:

Multiwavelength images of the fifty-three galaxies of the final sample (MIPS-d+MIPS-u). The cut-outs have a size of 10'' $\times $ 10''. North is up, East is at left.

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\par\includegraphics[width=17.5cm,clip]{0603fg27.eps}
\end{figure} Figure 15:

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