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<!-- DOI: 10.1051/0004-6361/200912064 -->

<h2 class="sec">Online Material</h2>
<p></p>
<h2 class="sec"><a name="SECTION000100000000000000000"></a><A NAME="OnlineM"></A>
Appendix B: Online Material
</h2>
For comparision we show the calibrated rawdata together with the
baseline subtracted and smoothed spectra already shown in the
text. <div class="inset-old">
<table>
<tr><td><!-- init Label --><A NAME="fig:waterspectra"></A><!-- end Label--><A NAME="2683"></A><A NAME="figure2362" HREF="img110.png"><IMG SRC="Timg110.png" ALT="\begin{figure}\par\mbox{\includegraphics[width=7.5cm]{12064f17.ps} \hspace{2cm}
...
...20.ps} \hspace{2cm}
\includegraphics[width=7.5cm]{12064f12.ps} }
\end{figure}" HEIGHT="237" WIDTH="194"></A><!-- HTML Figure number: 17 -->
</td>
<td class="img-txt"><span class="bold">Figure B.1:</span><p>
This figure shows the L1448, HH211 and IC443-G spectra. The positions
are listed in Table&nbsp;<a href="/articles/aa/full_html/2009/45/aa12064-09/aa12064-09.html#tab:table1">1</a>.
All spectra on the right are smoothed to a resolution of 0.5&nbsp;
<!-- MATH: ${\rm km ~ s^{-1}}$ --><IMG SRC="img26.png" ALT="${\rm km ~ s^{-1}}$" ALIGN="MIDDLE" BORDER="0" HEIGHT="30" WIDTH="41">
and clipped for clarity. These spectra are also calibrated in
frequency. The spectra on the left are the calibrated rawdata with a
zero order baseline subtraction. For strip maps, a letter in the upper
right corner indicates in which part of the flow the spectra has been
collected (R&nbsp;=&nbsp;red, B&nbsp;=&nbsp;blue and
C&nbsp;=&nbsp;center).
</td>
</tr><tr><td colspan="2"><a href="http://dexter.edpsciences.org/applet.php?pdf_id=17&DOI=10.1051/0004-6361/200912064" target="DEXTER">Open with DEXTER</a></td></tr>

</table></div>
<p></p><div class="inset-old">
<table>
<tr><td><!-- init Label --><A NAME="fig:waterspectra2"></A><!-- end Label--><A NAME="2687"></A><A NAME="figure2376" HREF="img111.png"><IMG SRC="Timg111.png" ALT="\begin{figure}
\par\mbox{\includegraphics[width=7.5cm]{12064f21.ps} \hspace{2cm}...
...24.ps} \hspace{2cm}
\includegraphics[width=7.5cm]{12064f25.ps} }
\end{figure}" HEIGHT="237" WIDTH="195"></A><!-- HTML Figure number: 18 -->
</td>
<td class="img-txt"><span class="bold">Figure B.2:</span><p>
The same as Fig.&nbsp;<a href="/articles/aa/full_html/2009/45/aa12064-09/aa12064-09.html#fig:waterspectra">B.1</a>
but for L1551, Sa136 and TW&nbsp;Hya.
</td>
</tr><tr><td colspan="2"><a href="http://dexter.edpsciences.org/applet.php?pdf_id=18&DOI=10.1051/0004-6361/200912064" target="DEXTER">Open with DEXTER</a></td></tr>

</table></div>
<p></p><div class="inset-old">
<table>
<tr><td><!-- init Label --><A NAME="fig:waterspectra3"></A><!-- end Label--><A NAME="2693"></A><A NAME="figure2390" HREF="img112.png"><IMG SRC="Timg112.png" ALT="\begin{figure}\par\mbox{\includegraphics[width=7.5cm]{12064f26.ps} \hspace{2cm}
...
...f33.ps} \hspace{2cm}
\includegraphics[width=7.5cm]{12064f8.ps} }
\end{figure}" HEIGHT="208" WIDTH="195"></A><!-- HTML Figure number: 19 -->
</td>
<td class="img-txt"><span class="bold">Figure B.3:</span><p>
The same as Fig.&nbsp;<a href="/articles/aa/full_html/2009/45/aa12064-09/aa12064-09.html#fig:waterspectra">B.1</a>
but for eps Cha&nbsp; <small>I&nbsp;</small>N,
HH54 B, G327.3-0.6, NGC&nbsp;6334&nbsp; <small>I</small>
and Ser&nbsp;SMM1.
</td>
</tr><tr><td colspan="2"><a href="http://dexter.edpsciences.org/applet.php?pdf_id=19&DOI=10.1051/0004-6361/200912064" target="DEXTER">Open with DEXTER</a></td></tr>

</table></div>
<p></p><div class="inset-old">
<table>
<tr><td><!-- init Label --><A NAME="fig:waterspectra4"></A><!-- end Label--><A NAME="2698"></A><A NAME="figure2412" HREF="img113.png"><IMG SRC="Timg113.png" ALT="\begin{figure}\par\mbox{\includegraphics[width=7cm]{12064f34.ps} \hspace{2cm}
\...
...4f39.ps} \hspace{2cm}
\includegraphics[width=7cm]{12064f10.ps} }
\end{figure}" HEIGHT="233" WIDTH="185"></A><!-- HTML Figure number: 20 -->
</td>
<td class="img-txt"><span class="bold">Figure B.4:</span><p>
The same as Fig.&nbsp;<a href="/articles/aa/full_html/2009/45/aa12064-09/aa12064-09.html#fig:waterspectra">B.1</a>
but for 3C391 BML, B335, NGC&nbsp;7538 IRS1 and L1157. For L1157,
the AC2 data are plotted in gray and the AOS data in black.
</td>
</tr><tr><td colspan="2"><a href="http://dexter.edpsciences.org/applet.php?pdf_id=20&DOI=10.1051/0004-6361/200912064" target="DEXTER">Open with DEXTER</a></td></tr>

</table></div>
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