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<title>CASA Scripts &amp; Data</title>

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&nbsp;<a class="navig" href="http://www.nrao.edu/">NRAO Home</a> &gt;
<a class="navig" href="http://casa.nrao.edu/">CASA</a> &gt; Scripts &amp; Data

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<p><a class="leftmenu" href="#docs">Documentation and Help</a></p>
<ul>
<li><p><a class="leftmenu" href="./casahelp.shtml">Getting Help</a></p>
<li><p><a class="leftmenu" href="./gettingstarted.shtml">Getting Started</a></p>
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<li><p><a class="leftmenu" href="http://casa.nrao.edu/docs/casaref/CasaRef.html">Toolkit Manual</a></p>
<li><p><a class="leftmenu" href="http://casa.nrao.edu/docs/taskref/TaskRef.html">Task Reference</a></p>
</ul>

<p><a class="leftmenu" href="#scripts">Training, Scripts, Data</a></p>
<ul>
<li><p><a class="leftmenu" href="./casatraining.shtml">CASA Training</a></p>
<li><p><a class="leftmenu" href="http://casa.nrao.edu/Data">CASA Data Archive</a></p>
<li><p><a class="leftmenu" href="./Doc/Scripts/">CASA Script Archive</a></p>
</ul>

<p><A class="leftmenu" HREF="https://wikio.nrao.edu/bin/view/ALMA/SimulatorCookbook">
    ALMA Simulator</A></p>
<p><a class="leftmenu" href="http://casa.nrao.edu/CasaViewerDemo/casaViewerDemo.html">Viewer Demo</a></p>

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<p><A NAME="scripts">
<big><b>CASA Scripts and Data</b></big>

<P>As part of our testing and training programs, we have developed a
number of "use case" and "demo" scripts.  Here are links to a
selection of these:
</P>

<ul>
<li>VLA HI Line Data (NGC5921)<A NAME="n5921">

  <P>This is a relatively small dataset suitable for a quick demo.</P>

  <P>
  <table cellspacing=0 cellpadding=1 border=0 width=100%>
  <tr><td align=left valign=top width=66%>
  <font face=helvetica size="+1">
  <ul>
  <li>The data is packaged with CASA, no need to download
  <li><A HREF="Doc/Scripts/ngc5921_demo.py">
      NGC5921 Demo Script</A> (casapy script)
  <li><A HREF="http://casa.nrao.edu/Images/n5921mom01.png">
      NGC5921 Moment 0/1 Image</A> (PNG 20KB)
  </ul>
  </font>
  <br>
  <i>At right:</i> 
  Integrated VLA HI line intensity image (false color) with HI
  velocity field superposed (contours) for the galaxy NGC5921.
  </td><td align=right>
  <img src="http://casa.nrao.edu/Images/n5921mom01-small.png" border=0 alt="NGC5921">
  </td></tr>
  </table>
  </P>

<li>VLA HI Line Data (NGC2403)<A NAME="n2403">

  <P>This is a larger dataset (the MS will be 5.2GB) and it will take 
     longer to run (~40m) but produces a much nicer image.</P>

  <P>
  <table cellspacing=0 cellpadding=1 border=0 width=100%>
  <tr><td align=left valign=top width=66%>
  <font face=helvetica size="+1">
  <ul>
  <li><A HREF="http://casa.nrao.edu/Data/VLA/NGC2403/ngc2403data.tgz">
      NGC2403 data</A> (tar-gzipped VLAExport 513MB)
  <li><A HREF="Doc/Scripts/ngc2403_tutorial.py">
      NGC2403 Tutorial Script</A> (casapy script)
  <li><A HREF="http://casa.nrao.edu/Images/n2403mom0.png">
      NGC2403 Moment 0 Image</A> (PNG 183KB)
  </ul>
  </font>
  <br>
  <i>At right:</i> 
  Integrated VLA HI line intensity greyscale image (from moment zero
  map) of the galaxy NGC2403.
  </td><td align=right>
  <img src="http://casa.nrao.edu/Images/n2403mom0-small.png" border=0 alt="NGC2403">
  </td></tr>
  </table>
  </P>

<li>BIMA CO Line Data (NGC4826)<A NAME="n4826">

  <P>This is a 3mm CO line mosaic from the BIMA SONG survey
     (Helfer, Thornley, Regan, et al., 2003, ApJS, 145, 259).</P>

  <P>
  <table cellspacing=0 cellpadding=1 border=0 width=100%>
  <tr><td align=left valign=top width=66%>
  <font face=helvetica size="+1">
  <ul>
  <li><A HREF="http://casa.nrao.edu/Data/BIMA/NGC4826/ngc4826.fitsfiles.tgz">
      NGC4826 data</A> (tar-gzipped UVFITS 66MB)
  <li><A HREF="Doc/Scripts/ngc4826_tutorial.py">
      NGC4826 Tutorial Script</A> (casapy script)
  <li><A HREF="http://casa.nrao.edu/Images/n4826mom1.png">
      NGC4826 Moment 1 Image</A> (PNG 183KB)
  </ul>
  </font>
  <br>
  <i>At right:</i> 
  False-color image of the CO velocity field (from a moment 1 image)
  for the BIMA SONG galaxy NGC4826.
  </td><td align=right>
  <img src="http://casa.nrao.edu/Images/n4826mom1-small.png" border=0 alt="NGC4826">
  </td></tr>
  </table>
  </P>

<li>VLA 3.6cm Continuum (CLASS B1608+656)<A NAME="b1608">

  <P>This is a 3.6cm VLA continuum dataset taken in 1995 as
     follow up to the CLASS gravitational lens survey
     (S.T. Myers et al., 1995, ApJL, 447, L5).  
     This is a small dataset suitable for quick demos.</P>

  <P>
  <table cellspacing=0 cellpadding=1 border=0 width=100%>
  <tr><td align=left valign=top width=66%>
  <font face=helvetica size="+1">
  <ul>
  <li><A HREF="http://casa.nrao.edu/Data/VLA/B1608+656/AM484_B950818.xp1">
      B1608+656 VLA data</A> (VLAExport 3.4MB)
  <li><A HREF="Doc/Scripts/b1608_demo.py">
      B1608+656 Demo Script</A> (casapy script)
  <li><A HREF="http://casa.nrao.edu/Images/b1608_950818.png">
      B1608+656 3.6cm Image</A> (PNG 31KB)
  </ul>
  </font>
  <br>
  <i>At right:</i> 
  Continuum image of 4-image "quad" gravitational lens system CLASS 
  B1608+656 from a 5-minute VLA 3.6cm snapshot.
  </td><td align=right>
  <img src="http://casa.nrao.edu/Images/b1608_950818-small.png" border=0 alt="CLASS B1608+656">
  </td></tr>
  </table>
  </P>

<li>VLA 6cm Continuum Polarization (Jupiter)<A NAME="jupiter">

  <P>This is a 6cm VLA continuum polarimetry dataset taken in 1999 as
     part of the VLA flux calibration test program.</P>

  <P>
  <table cellspacing=0 cellpadding=1 border=0 width=100%>
  <tr><td align=left valign=top width=66%>
  <font face=helvetica size="+1">
  <ul>
  <li><A HREF="http://casa.nrao.edu/Data/VLA/Planets6cm/planets_6cm.fits">
      Jupiter/FLUX99 VLA data</A> (UVFITS 129MB)
  <li><A HREF="Doc/Scripts/jupiter6cm_demo.py">
      Jupiter Tutorial/Demo Script</A> (casapy script)
  <li><A HREF="http://casa.nrao.edu/Images/jupiter6cmPol.png">
      Jupiter 6cm Polarization Image</A> (PNG 24KB)
  </ul>
  </font>
  <br>
  <i>At right:</i> 
  Image of Jupiter 6cm intensity (false color) with polarized intensity 
  (yellow contours) and
  polarization vectors (white, rotated 90deg to show B-field direction).
  </td><td align=right>
  <img src="http://casa.nrao.edu/Images/jupiter6cmPol-small.png" border=0 alt="Jupiter">
  </td></tr>
  </table>
  </P>

<li>VLA 6cm Continuum Polarimetry (3C129)<A NAME="3c129">

  <P>This is a larger dataset (the raw data is 107MB) and it will take 
     longer to run (~40m).  This combines B and C configuration data
     as 3C129 has a lot of large-scale emission.  This makes a nice
     image.</P>

  <P>
  <table cellspacing=0 cellpadding=1 border=0 width=100%>
  <tr><td align=left valign=top width=66%>
  <font face=helvetica size="+1">
  <ul>
  <li><A HREF="http://casa.nrao.edu/Data/VLA/3C129/3c129data.tgz">
      3C129 data</A> (tar-gzipped VLAExport 107MB)
  <li><A HREF="Doc/Scripts/3c129_tutorial.py">
      3C129 Tutorial Script</A> (casapy script)
  <li><A HREF="http://casa.nrao.edu/Images/3c129Pol.png">
      3C129 Polarization Image</A> (PNG 63KB)
  </ul>
  </font>
  <br>
  <i>At right:</i> 
  Image of 3C129 6cm intensity (false color) with 
  polarization vectors (white, rotated 90deg to show B-field direction).
  </td><td align=right>
  <img src="http://casa.nrao.edu/Images/3c129Pol-small.png" border=0 alt="3C129">
  </td></tr>
  </table>
  </P>

</ul>
</p>

<p><A NAME="expert">
<big><b>For Experienced Users: CASA Scripts and Data</b></big>

<P>Here are some more data and scripts, intended for more experienced
CASA users and exploring more technical uses of the package.   These 
scripts are not generally set up as demos or tutorials, and users will
likely need to read through them carefully and in some cases
cut-and-paste commands to their casapy session.
</P>

<ul>
<li>SMA CO Line Data (G19.3+0.07)<A NAME="sma">

  <P>This is a SMA dataset with a large number of spectral channels.</P>

  <P>
  <table cellspacing=0 cellpadding=1 border=0 width=100%>
  <tr><td align=left valign=top width=66%>
  <font face=helvetica size="+1">
  <ul>
  <li><A HREF="http://casa.nrao.edu/Data/SMA/spw_fits_files.tar">
      SMA data</A> (tar UVFITS 891MB)
  <li><A HREF="Doc/Scripts/sma_reduction_example.py">
      SMA example script</A> (casapy script)
  <li><A HREF="http://casa.nrao.edu/Images/g19_COint.png">
      SMA on Spitzer Image</A> (PNG 60KB)
  </ul>
  </font>
  <br>
  <i>At right:</i> 
  Spitzer GLIMPSE 8 um image with green contours showing the integrated CO(2-1) emission
  from SMA for infrared dark cloud G19.3+0.07 (Brogan et al. in prep).
  </td><td align=right>
  <img src="http://casa.nrao.edu/Images/g19_COint-small.png" border=0 alt="G19 CO">
  </td></tr>
  </table>
  </P>

</ul>
</p>

<p><A NAME="sessions">
<big><b>CASA Training Materials</b></big>

<P>We have held a number of training sessions for CASA.  We intend
to archive the materials here for use online for training, and for
building new training sessions.  These are available from the
<a href="./casatraining.shtml">CASA Training Page</a>
</P>

<p><A NAME="docs">
<big><b>CASA Documentation and Help</b></big>

<P>There are a number of reference documents and help facilities
available to the user, for more information, see the
<A HREF="./casahelp.shtml">Help and Documentation</A> page.
</P>

<p>

<hr>

<p>
<small>
<i>
Please send any comments or questions about <font
            face=helvetica>CASA</font>
to <a href="mailto:casa-request@nrao.edu">casa-request@nrao.edu</a><p>

Copyright &#169; 1995-2007 Associated Universities Inc.,
Washington, D.C.</i>
<p>
<i>
<a href="http://www.gnu.org/copyleft/gpl.html">This code is available
under the terms of the GNU General Public Lincense</a>

</small>

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<em>Modified on 
Wednesday, 30-Mar-2022 16:40:28 EDT
</em>

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