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<div class="section" id="virtual-observatory">
<h1>Virtual Observatory<a class="headerlink" href="#virtual-observatory" title="Permalink to this headline">¶</a></h1>
<p>The <a class="reference external" href="https://github.com/python4vo/coatpy">COATpy</a> wrapping of <a class="reference external" href="https://code.google.com/p/pyvolib">pyvolib</a> exposes a number of different virtual
observatory tools. We will go over each of these in turn.</p>
<div class="contents local topic" id="contents">
<ul class="simple">
<li><a class="reference internal" href="#name-position-resolver" id="id1">Name Position Resolver</a></li>
<li><a class="reference internal" href="#catalog-search" id="id2">Catalog Search</a></li>
<li><a class="reference internal" href="#image-search" id="id3">Image Search</a></li>
</ul>
</div>
<div class="section" id="name-position-resolver">
<h2><a class="toc-backref" href="#id1">Name Position Resolver</a><a class="headerlink" href="#name-position-resolver" title="Permalink to this headline">¶</a></h2>
<div class="sidebar">
<p class="first sidebar-title">Names of things</p>
<p>Presently the “names” of things have to be URL encoded or the tool
will not resolve. Use <code class="docutils literal"><span class="pre">IC+348</span></code> or <code class="docutils literal"><span class="pre">IC348</span></code> instead of <code class="docutils literal"><span class="pre">IC</span> <span class="pre">348</span></code>.
Programmatically this looks like:</p>
<div class="highlight-python"><div class="highlight"><pre><span></span><span class="n">urllib</span><span class="o">.</span><span class="n">quote_plus</span><span class="p">(</span><span class="s2">"IC 348"</span><span class="p">)</span>
</pre></div>
</div>
<p class="last">This will be fixed in an upcoming update.</p>
</div>
<p><code class="docutils literal"><span class="pre">Sesame</span></code> is a basic name resolver that returns the position of objects as a
tuple. You can specify which service you wish to use:</p>
<div class="highlight-python"><div class="highlight"><pre><span></span><span class="kn">from</span> <span class="nn">coatpy</span> <span class="kn">import</span> <span class="n">Sesame</span>
<span class="n">simbad</span> <span class="o">=</span> <span class="n">Sesame</span><span class="p">(</span><span class="n">opt</span><span class="o">=</span><span class="s1">'S'</span><span class="p">)</span>
<span class="n">ned</span> <span class="o">=</span> <span class="n">Sesame</span><span class="p">(</span><span class="n">opt</span><span class="o">=</span><span class="s1">'N'</span><span class="p">)</span>
<span class="n">ned</span><span class="o">.</span><span class="n">resolve</span><span class="p">(</span><span class="s1">'M51'</span><span class="p">)</span>
<span class="c1"># the services do not agree; doing this will produce an exception.</span>
<span class="k">assert</span> <span class="n">simbad</span><span class="o">.</span><span class="n">resolve</span><span class="p">(</span><span class="s1">'IC348'</span><span class="p">)</span> <span class="o">==</span> <span class="n">ned</span><span class="o">.</span><span class="n">resolve</span><span class="p">(</span><span class="s1">'IC348'</span><span class="p">)</span>
</pre></div>
</div>
</div>
<div class="section" id="catalog-search">
<h2><a class="toc-backref" href="#id2">Catalog Search</a><a class="headerlink" href="#catalog-search" title="Permalink to this headline">¶</a></h2>
<p>The <code class="docutils literal"><span class="pre">ConeSearch</span></code> tool is a standardized interface to one of hundreds of
catalogs. The necessary parameters are:</p>
<ul class="simple">
<li><code class="docutils literal"><span class="pre">RA</span></code>: decimal degrees</li>
<li><code class="docutils literal"><span class="pre">DEC</span></code>: decimal degrees</li>
<li><code class="docutils literal"><span class="pre">SR</span></code>: cone radius in decimal degrees</li>
</ul>
<p>An optional parameter <code class="docutils literal"><span class="pre">VERB</span></code> varies the verbosity of the query response.</p>
<div class="sidebar">
<p class="first sidebar-title">Verbs</p>
<p class="last">Only <code class="docutils literal"><span class="pre">VERB=1</span></code> is standardized across all catalogs. A <code class="docutils literal"><span class="pre">VERB=1</span></code> query
returns only the positions of objects found the queried catalog.
<code class="docutils literal"><span class="pre">VERB=2</span></code> returns the “default” set of columns chosen by the
archive. <code class="docutils literal"><span class="pre">VERB=3</span></code> returns all columns. Not all services respond
to <code class="docutils literal"><span class="pre">VERB</span></code> parameters.</p>
</div>
<p>As with the web queries you can wrap up the parameters in a dictionary:</p>
<div class="highlight-python"><div class="highlight"><pre><span></span><span class="kn">from</span> <span class="nn">coatpy</span> <span class="kn">import</span> <span class="n">ConeSearch</span><span class="p">,</span> <span class="n">Sesame</span>
<span class="n">simbad</span> <span class="o">=</span> <span class="n">Sesame</span><span class="p">(</span><span class="n">opt</span><span class="o">=</span><span class="s1">'S'</span><span class="p">)</span>
<span class="n">params</span> <span class="o">=</span> <span class="p">{}</span>
<span class="n">params</span><span class="p">[</span><span class="s1">'RA'</span><span class="p">]</span> <span class="o">=</span> <span class="n">simbad</span><span class="o">.</span><span class="n">resolve</span><span class="p">(</span><span class="s2">"IC348"</span><span class="p">)[</span><span class="mi">0</span><span class="p">]</span>
<span class="n">params</span><span class="p">[</span><span class="s1">'DEC'</span><span class="p">]</span> <span class="o">=</span> <span class="n">simbad</span><span class="o">.</span><span class="n">resolve</span><span class="p">(</span><span class="s2">"IC348"</span><span class="p">)[</span><span class="mi">1</span><span class="p">]</span>
<span class="n">params</span><span class="p">[</span><span class="s1">'SR'</span><span class="p">]</span> <span class="o">=</span> <span class="mf">1.</span><span class="o">/</span><span class="mf">60.</span>
<span class="n">params</span><span class="p">[</span><span class="s1">'VERB'</span><span class="p">]</span> <span class="o">=</span> <span class="mi">3</span>
</pre></div>
</div>
<div class="sidebar">
<p class="first sidebar-title">Discovering catalogs</p>
<p class="last">At this point the system breaks down a little bit as we are not providing
a programmatic tool for discovering catalogs. You have to use an online
<a class="reference external" href="http://nvo.stsci.edu/vor10/index.aspx">Directory</a> to search the catalogs you want. <a class="reference external" href="http://nvo.stsci.edu/vor10/index.aspx#Table||query_string=IC%20348">Here is an example
Directory search.</a> Once a catalog is found, you want to copy the
“accessURL” from the search table or open the “Full Record” and open the
“Simple Cone Search” option. <a class="reference external" href="http://nvo.stsci.edu/vor10/getRecord.aspx?id=ivo://CDS.VizieR/J/AJ/122/866">Here is the catalog used in this example.</a></p>
</div>
<p>enter the query URL for the target catalog (see sidebar), and create a catalog
handler <code class="docutils literal"><span class="pre">ic348cxo</span></code> that wraps the query tool. We use the <code class="docutils literal"><span class="pre">getRaw</span></code> function
of the ConeSearch to retrieve the raw string result that we then dump into a
file and extract back the data using <a class="reference external" href="http://astropy.org">astropy</a>:</p>
<div class="highlight-python"><div class="highlight"><pre><span></span><span class="kn">from</span> <span class="nn">astropy.table</span> <span class="kn">import</span> <span class="n">Table</span>
<span class="n">url</span> <span class="o">=</span> <span class="s2">"http://vizier.u-strasbg.fr/viz-bin/votable/-A?-source=J/AJ/122/866&"</span>
<span class="n">ic348cxo</span> <span class="o">=</span> <span class="n">ConeSearch</span><span class="p">(</span><span class="n">url</span><span class="p">)</span>
<span class="k">with</span> <span class="nb">open</span><span class="p">(</span><span class="s1">'ic348cxo.xml'</span><span class="p">,</span><span class="s1">'wb'</span><span class="p">)</span> <span class="k">as</span> <span class="n">f</span><span class="p">:</span>
<span class="n">f</span><span class="o">.</span><span class="n">write</span><span class="p">(</span><span class="n">ic348cxo</span><span class="o">.</span><span class="n">getRaw</span><span class="p">(</span><span class="o">**</span><span class="n">params</span><span class="p">))</span>
<span class="n">data</span> <span class="o">=</span> <span class="n">Table</span><span class="o">.</span><span class="n">read</span><span class="p">(</span><span class="n">f</span><span class="o">.</span><span class="n">name</span><span class="p">,</span> <span class="n">format</span><span class="o">=</span><span class="s1">'votable'</span><span class="p">)</span>
</pre></div>
</div>
</div>
<div class="section" id="image-search">
<h2><a class="toc-backref" href="#id3">Image Search</a><a class="headerlink" href="#image-search" title="Permalink to this headline">¶</a></h2>
<p><code class="docutils literal"><span class="pre">Siap</span></code> is the tool for querying image services is:</p>
<div class="highlight-python"><div class="highlight"><pre><span></span><span class="kn">from</span> <span class="nn">coatpy</span> <span class="kn">import</span> <span class="n">Siap</span>
</pre></div>
</div>
<p>The <code class="docutils literal"><span class="pre">Siap</span></code> acronym stands for <em>Simple Image Access Protocol</em> and as with
<code class="docutils literal"><span class="pre">ConeSearch</span></code> the inputs are fairly simple:</p>
<ul class="simple">
<li><code class="docutils literal"><span class="pre">RA</span></code>: Decimal Degrees</li>
<li><code class="docutils literal"><span class="pre">DEC</span></code>: Decimal Degrees</li>
<li><code class="docutils literal"><span class="pre">SIZE</span></code>: An image size in degrees</li>
<li><code class="docutils literal"><span class="pre">FORMAT</span></code>: [Optional] default: image/fits (or image/jpeg)</li>
</ul>
<div class="admonition note">
<p class="first admonition-title">Note</p>
<p class="last">Various image archives have appended other query parameters onto
the SIAP standard to provide additional initial filtering of the images
returned. A good example is the <a class="reference external" href="http://irsa.ipac.caltech.edu/applications/2MASS/IM/docs/siahelp.html">IRSA 2MASS</a>
service. The <code class="docutils literal"><span class="pre">Siap</span></code> tool currently throws Exceptions on extra parameters.</p>
</div>
<div class="admonition-exercise-find-hst-images-of-a-young-cluster admonition">
<p class="first admonition-title">Exercise: find HST images of a young cluster</p>
<p>In this exercise we will go through the steps necessary for downloading
images with <code class="docutils literal"><span class="pre">Siap</span></code> from the Hubble Legacy Archive.</p>
<p>The first step is to set up the query, which is nearly identical to the
previous examples.</p>
<div class="highlight-python"><div class="highlight"><pre><span></span><span class="kn">import</span> <span class="nn">urllib2</span>
<span class="kn">from</span> <span class="nn">coatpy</span> <span class="kn">import</span> <span class="n">Siap</span><span class="p">,</span> <span class="n">Sesame</span>
<span class="kn">import</span> <span class="nn">vo</span>
<span class="n">simbad</span> <span class="o">=</span> <span class="n">Sesame</span><span class="p">(</span><span class="n">opt</span><span class="o">=</span><span class="s2">"S"</span><span class="p">)</span>
<span class="n">url</span> <span class="o">=</span> <span class="s2">" http://hla.stsci.edu/cgi-bin/acsSIAP.cgi?strict=1"</span>
<span class="n">hla</span> <span class="o">=</span> <span class="n">Siap</span><span class="p">(</span><span class="n">url</span><span class="p">)</span>
<span class="n">params</span> <span class="o">=</span> <span class="p">{}</span>
<span class="n">position</span> <span class="o">=</span> <span class="n">simbad</span><span class="o">.</span><span class="n">resolve</span><span class="p">(</span><span class="s1">'IC348'</span><span class="p">)</span>
<span class="n">params</span><span class="o">.</span><span class="n">update</span><span class="p">(</span><span class="nb">zip</span><span class="p">((</span><span class="s1">'RA'</span><span class="p">,</span> <span class="s1">'DEC'</span><span class="p">),</span> <span class="n">position</span><span class="p">))</span>
<span class="n">params</span><span class="p">[</span><span class="s1">'SIZE'</span><span class="p">]</span> <span class="o">=</span> <span class="mf">1.</span><span class="o">/</span><span class="mf">60.</span>
<span class="n">params</span><span class="p">[</span><span class="s1">'FORMAT'</span><span class="p">]</span> <span class="o">=</span> <span class="s1">'image/fits'</span>
<span class="k">with</span> <span class="nb">open</span><span class="p">(</span><span class="s1">'hla_ic348_images.xml'</span><span class="p">,</span> <span class="s1">'wb'</span><span class="p">)</span> <span class="k">as</span> <span class="n">f</span><span class="p">:</span>
<span class="n">f</span><span class="o">.</span><span class="n">write</span><span class="p">(</span><span class="n">hla</span><span class="o">.</span><span class="n">getRaw</span><span class="p">(</span><span class="o">**</span><span class="n">params</span><span class="p">))</span>
</pre></div>
</div>
<p>The main difference between a catalog and an image query is that an image
query results in a series of <strong>pointers</strong> to the image files that can be
examined and filtered before the reference files are downloaded. We use
the <a class="reference external" href="http://stsdas.stsci.edu/astrolib/vo/html/">vo</a> module to parse the
results, extracting the table of images that satisfy our query.</p>
<div class="highlight-python"><div class="highlight"><pre><span></span><span class="n">vot</span> <span class="o">=</span> <span class="n">vo</span><span class="o">.</span><span class="n">table</span><span class="o">.</span><span class="n">parse_single_table</span><span class="p">(</span><span class="s1">'hla_ic348_images.xml'</span><span class="p">)</span>
<span class="n">image_table</span> <span class="o">=</span> <span class="n">vot</span><span class="o">.</span><span class="n">array</span>
</pre></div>
</div>
<p>The returned array contains <strong>66</strong> fields!</p>
<div class="highlight-python"><div class="highlight"><pre><span></span><span class="k">print</span><span class="p">(</span><span class="n">image_table</span><span class="o">.</span><span class="n">dtype</span><span class="o">.</span><span class="n">names</span><span class="p">)</span>
</pre></div>
</div>
<p>If all we want is the actual data then the important column is <strong>URL</strong>
while the <strong>filename</strong> column is also useful.</p>
<div class="highlight-python"><div class="highlight"><pre><span></span><span class="c1"># just grab the first image returned</span>
<span class="n">image</span> <span class="o">=</span> <span class="n">image_table</span><span class="p">[</span><span class="mi">0</span><span class="p">]</span>
<span class="n">image_url</span> <span class="o">=</span> <span class="n">image</span><span class="p">[</span><span class="s1">'URL'</span><span class="p">]</span>
<span class="n">filename</span> <span class="o">=</span> <span class="n">image</span><span class="p">[</span><span class="s1">'filename'</span><span class="p">]</span> <span class="o">+</span> <span class="s1">'.fits'</span>
<span class="k">with</span> <span class="nb">open</span><span class="p">(</span><span class="n">filename</span><span class="p">,</span> <span class="s1">'wb'</span><span class="p">)</span> <span class="k">as</span> <span class="n">image_file</span><span class="p">:</span>
<span class="n">image_handler</span> <span class="o">=</span> <span class="n">urllib2</span><span class="o">.</span><span class="n">urlopen</span><span class="p">(</span><span class="n">image_url</span><span class="p">)</span>
<span class="n">image_file</span><span class="o">.</span><span class="n">write</span><span class="p">(</span><span class="n">image_handler</span><span class="o">.</span><span class="n">read</span><span class="p">())</span>
<span class="n">image_handler</span><span class="o">.</span><span class="n">close</span><span class="p">()</span>
</pre></div>
</div>
<p class="last">Continue this exercise by examining the resulting image.</p>
</div>
<p class="flip9">Click to Show/Hide Solution</p> <div class="panel9"><p>We use <a class="reference external" href="http://docs.astropy.org/en/stable/io/fits/">astropy.io.fits</a> to open the image file and examine its contents.</p>
<div class="highlight-python"><div class="highlight"><pre><span></span><span class="kn">from</span> <span class="nn">astropy.io</span> <span class="kn">import</span> <span class="n">fits</span>
<span class="kn">import</span> <span class="nn">aplpy</span>
<span class="kn">import</span> <span class="nn">matplotlib.pyplot</span> <span class="kn">as</span> <span class="nn">plt</span>
<span class="n">hdulist</span> <span class="o">=</span> <span class="n">fits</span><span class="o">.</span><span class="n">open</span><span class="p">(</span><span class="n">filename</span><span class="p">)</span>
<span class="c1"># check for multiple FITS extensions and their contents</span>
<span class="c1"># in this case the "PRIMARY" header is empty</span>
<span class="k">for</span> <span class="n">hdu</span> <span class="ow">in</span> <span class="n">hdulist</span><span class="p">:</span>
<span class="k">print</span><span class="p">(</span><span class="s1">'name: {0} type: {1}'</span><span class="o">.</span><span class="n">format</span><span class="p">(</span><span class="n">hdu</span><span class="o">.</span><span class="n">name</span><span class="p">,</span> <span class="nb">type</span><span class="p">(</span><span class="n">hdu</span><span class="o">.</span><span class="n">data</span><span class="p">)))</span>
<span class="n">fig</span> <span class="o">=</span> <span class="n">plt</span><span class="o">.</span><span class="n">figure</span><span class="p">(</span><span class="n">figsize</span><span class="o">=</span><span class="p">(</span><span class="mi">15</span><span class="p">,</span> <span class="mi">7</span><span class="p">))</span>
<span class="n">f1</span> <span class="o">=</span> <span class="n">aplpy</span><span class="o">.</span><span class="n">FITSFigure</span><span class="p">(</span><span class="n">filename</span><span class="p">,</span> <span class="n">hdu</span><span class="o">=</span><span class="mi">1</span><span class="p">,</span> <span class="n">subplot</span><span class="o">=</span><span class="p">[</span><span class="mf">0.1</span><span class="p">,</span><span class="mf">0.1</span><span class="p">,</span><span class="mf">0.3</span><span class="p">,</span><span class="mf">0.65</span><span class="p">],</span> <span class="n">figure</span><span class="o">=</span><span class="n">fig</span><span class="p">)</span>
<span class="n">f1</span><span class="o">.</span><span class="n">set_tick_labels_font</span><span class="p">(</span><span class="n">size</span><span class="o">=</span><span class="s1">'x-small'</span><span class="p">)</span>
<span class="n">f1</span><span class="o">.</span><span class="n">set_axis_labels_font</span><span class="p">(</span><span class="n">size</span><span class="o">=</span><span class="s1">'small'</span><span class="p">)</span>
<span class="n">f1</span><span class="o">.</span><span class="n">show_grayscale</span><span class="p">()</span>
<span class="n">f2</span> <span class="o">=</span> <span class="n">aplpy</span><span class="o">.</span><span class="n">FITSFigure</span><span class="p">(</span><span class="n">filename</span><span class="p">,</span> <span class="n">hdu</span><span class="o">=</span><span class="mi">2</span><span class="p">,</span> <span class="n">subplot</span><span class="o">=</span><span class="p">[</span><span class="mf">0.4</span><span class="p">,</span><span class="mf">0.1</span><span class="p">,</span><span class="mf">0.3</span><span class="p">,</span><span class="mf">0.65</span><span class="p">],</span> <span class="n">figure</span><span class="o">=</span><span class="n">fig</span><span class="p">)</span>
<span class="n">f2</span><span class="o">.</span><span class="n">hide_xaxis_label</span><span class="p">()</span>
<span class="n">f2</span><span class="o">.</span><span class="n">hide_xtick_labels</span><span class="p">()</span>
<span class="n">f2</span><span class="o">.</span><span class="n">hide_yaxis_label</span><span class="p">()</span>
<span class="n">f2</span><span class="o">.</span><span class="n">hide_ytick_labels</span><span class="p">()</span>
<span class="n">f2</span><span class="o">.</span><span class="n">show_colorscale</span><span class="p">()</span>
<span class="n">f3</span> <span class="o">=</span> <span class="n">aplpy</span><span class="o">.</span><span class="n">FITSFigure</span><span class="p">(</span><span class="n">filename</span><span class="p">,</span> <span class="n">hdu</span><span class="o">=</span><span class="mi">3</span><span class="p">,</span> <span class="n">subplot</span><span class="o">=</span><span class="p">[</span><span class="mf">0.7</span><span class="p">,</span><span class="mf">0.1</span><span class="p">,</span><span class="mf">0.3</span><span class="p">,</span><span class="mf">0.65</span><span class="p">],</span> <span class="n">figure</span><span class="o">=</span><span class="n">fig</span><span class="p">)</span>
<span class="n">f3</span><span class="o">.</span><span class="n">hide_xaxis_label</span><span class="p">()</span>
<span class="n">f3</span><span class="o">.</span><span class="n">hide_xtick_labels</span><span class="p">()</span>
<span class="n">f3</span><span class="o">.</span><span class="n">hide_yaxis_label</span><span class="p">()</span>
<span class="n">f3</span><span class="o">.</span><span class="n">hide_ytick_labels</span><span class="p">()</span>
<span class="n">f3</span><span class="o">.</span><span class="n">show_colorscale</span><span class="p">(</span><span class="n">cmap</span><span class="o">=</span><span class="s1">'spring'</span><span class="p">)</span>
</pre></div>
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