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<!-- DOI: 10.1051/0004-6361/201014693 -->

<h2 class="sec">Online Material</h2>

<p><A NAME="tab1"></A><p class="inset-old"><a href="/articles/aa/full_html/2010/10/aa14693-10/table1.html"><span class="bold">Table 1:</span></a>&#160;&#160;
Flux densities measured from the MIPS and <i> Herschel</i> maps.  </p>
<p></p><div class="inset-old">
<table>
<tr><td><!-- init Label --><A NAME="seds1"></A><!-- end Label--><A NAME="955"></A><A NAME="figure827" HREF="img33.png"><IMG SRC="Timg33.png" ALT="\begin{figure}
\par\includegraphics[width=17.5cm,clip]{f3_14693.eps}
\end{figure}" HEIGHT="196" WIDTH="197"></A><!-- HTML Figure number: 3 -->
</td>
<td class="img-txt"><span class="bold">Figure 3:</span><p>
SED template fits to HLS1-HLS9. The data points have been de-magnified
according to our lensing models of the foreground cluster. These
magnification factors can be found in Table&nbsp;<a href="/articles/aa/full_html/2010/10/aa14693-10/aa14693-10.html#tab2">2</a>.
The solid lines show the best-fit R09 template (in&nbsp;blue) and CE01
template (in&nbsp;red) to the FIR-mm data, excluding the 24&nbsp;<IMG SRC="img3.png" ALT="$\mu $" ALIGN="MIDDLE" BORDER="0" HEIGHT="26" WIDTH="11">m point.  LABOCA 870&nbsp;<IMG SRC="img3.png" ALT="$\mu $" ALIGN="MIDDLE" BORDER="0" HEIGHT="26" WIDTH="11">m and AzTEC 1.1&nbsp;mm
data are used to constrain these fits when the detection is of &gt;3-<IMG SRC="img5.png" ALT="$\sigma $" ALIGN="MIDDLE" BORDER="0" HEIGHT="26" WIDTH="13">
significance.  However, only the MIPS and <i> Herschel</i> data are shown in the figure. The dotted lines show the respective fits based solely on the observed 24&nbsp;<IMG SRC="img3.png" ALT="$\mu $" ALIGN="MIDDLE" BORDER="0" HEIGHT="26" WIDTH="11">m
point. Although both the R09 and the CE01 templates generally predict
reasonable values for the IR luminosity based on observed 24&nbsp;<IMG SRC="img3.png" ALT="$\mu $" ALIGN="MIDDLE" BORDER="0" HEIGHT="26" WIDTH="11">m emission, the&nbsp;24&nbsp;<IMG SRC="img3.png" ALT="$\mu $" ALIGN="MIDDLE" BORDER="0" HEIGHT="26" WIDTH="11">m-predicted SEDs typically do not provide reasonable fits to the FIR-mm&nbsp;data.
</td>
</tr><tr><td colspan="2"><a href="http://dexter.edpsciences.org/applet.php?pdf_id=3&DOI=10.1051/0004-6361/201014693" target="DEXTER">Open with DEXTER</a></td></tr>

</table></div>
<p></p><div class="inset-old">
<table>
<tr><td><!-- init Label --><A NAME="seds2"></A><!-- end Label--><A NAME="956"></A><A NAME="figure837" HREF="img34.png"><IMG SRC="Timg34.png" ALT="\begin{figure}
\par\includegraphics[width=17.5cm,clip]{f4_14693.eps}
\end{figure}" HEIGHT="196" WIDTH="197"></A><!-- HTML Figure number: 4 -->
</td>
<td class="img-txt"><span class="bold">Figure 4:</span><p>
SED template fits to HLS10-HLS19. The data points have been
de-magnified according to our lensing models of the foreground cluster.
These magnification factors can be found in Table&nbsp;<a href="/articles/aa/full_html/2010/10/aa14693-10/aa14693-10.html#tab2">2</a>.
The solid lines show the best-fit R09 template (in blue) and CE01
template (in&nbsp;red) to the FIR-mm data, excluding the 24&nbsp;<IMG SRC="img3.png" ALT="$\mu $" ALIGN="MIDDLE" BORDER="0" HEIGHT="26" WIDTH="11">m point.  LABOCA 870&nbsp;<IMG SRC="img3.png" ALT="$\mu $" ALIGN="MIDDLE" BORDER="0" HEIGHT="26" WIDTH="11">m and AzTEC 1.1&nbsp;mm
data are used to constrain these fits when the detection is of &gt;3-<IMG SRC="img5.png" ALT="$\sigma $" ALIGN="MIDDLE" BORDER="0" HEIGHT="26" WIDTH="13">
significance.  However, only the MIPS and <i> Herschel</i> data are shown in the figure. The dotted lines show the respective fits based solely on the observed 24&nbsp;<IMG SRC="img3.png" ALT="$\mu $" ALIGN="MIDDLE" BORDER="0" HEIGHT="26" WIDTH="11">m
point. Although both the R09 and the CE01 templates generally predict
reasonable values for the IR&nbsp;luminosity based on observed 24&nbsp;<IMG SRC="img3.png" ALT="$\mu $" ALIGN="MIDDLE" BORDER="0" HEIGHT="26" WIDTH="11">m emission, the&nbsp;24&nbsp;<IMG SRC="img3.png" ALT="$\mu $" ALIGN="MIDDLE" BORDER="0" HEIGHT="26" WIDTH="11">m-predicted SEDs typically do not provide reasonable fits to the FIR-mm&nbsp;data.
</td>
</tr><tr><td colspan="2"><a href="http://dexter.edpsciences.org/applet.php?pdf_id=4&DOI=10.1051/0004-6361/201014693" target="DEXTER">Open with DEXTER</a></td></tr>

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