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<li><a class="reference internal" href="#">pixtosky: Coordinate transformation to sky coordinates</a><ul>
<li><a class="reference internal" href="#parameters">PARAMETERS</a></li>
<li><a class="reference internal" href="#optional-parameters">Optional Parameters</a></li>
<li><a class="reference internal" href="#returns">RETURNS</a></li>
<li><a class="reference internal" href="#notes">NOTES</a></li>
<li><a class="reference internal" href="#usage">Usage</a></li>
<li><a class="reference internal" href="#examples">EXAMPLES</a></li>
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  <div class="section" id="pixtosky-coordinate-transformation-to-sky-coordinates">
<span id="pixtosky"></span><h1>pixtosky: Coordinate transformation to sky coordinates<a class="headerlink" href="#pixtosky-coordinate-transformation-to-sky-coordinates" title="Permalink to this headline">¶</a></h1>
<p>This task allows a user to perform coordinate transformations
with the full WCS and distortion model on source positions
from an input image to sky coordinates.  This task serves as
a replacement for the IRAF.STSDAS task &#8216;xy2rd&#8217;, albeit with the
added capability of understanding the full distortion model
provided in the headers of images updated for use with astrodrizzle and
tweakreg.</p>
<span class="target" id="module-drizzlepac.pixtosky"></span><p>pixtosky - A module to perform coordinate transformation from pixel to sky coordinates.</p>
<dl class="docutils">
<dt>License:</dt>
<dd><a class="reference external" href="http://www.stsci.edu/resources/software_hardware/pyraf/LICENSE">http://www.stsci.edu/resources/software_hardware/pyraf/LICENSE</a></dd>
</dl>
<div class="section" id="parameters">
<h2>PARAMETERS<a class="headerlink" href="#parameters" title="Permalink to this headline">¶</a></h2>
<dl class="docutils">
<dt>input <span class="classifier-delimiter">:</span> <span class="classifier">str</span></dt>
<dd>full filename with path of input image, an extension name [&#8216;sci&#8217;,1] should be
provided if input is a multi-extension FITS file</dd>
</dl>
</div>
<div class="section" id="optional-parameters">
<h2>Optional Parameters<a class="headerlink" href="#optional-parameters" title="Permalink to this headline">¶</a></h2>
<dl class="docutils">
<dt>x <span class="classifier-delimiter">:</span> <span class="classifier">float, optional</span></dt>
<dd>X position from input image</dd>
<dt>y <span class="classifier-delimiter">:</span> <span class="classifier">float, optional</span></dt>
<dd>Y position from input image</dd>
<dt>coords <span class="classifier-delimiter">:</span> <span class="classifier">str, optional</span></dt>
<dd>full filename with path of file with x,y coordinates</dd>
<dt>colnames <span class="classifier-delimiter">:</span> <span class="classifier">str, optional</span></dt>
<dd>comma separated list of column names from &#8216;coords&#8217; files
containing x,y coordinates, respectively. Will default to
first two columns if None are specified. Column names for ASCII
files will use &#8216;c1&#8217;,&#8217;c2&#8217;,... convention.</dd>
<dt>separator <span class="classifier-delimiter">:</span> <span class="classifier">str, optional</span></dt>
<dd>non-blank separator used as the column delimiter in the coords file</dd>
<dt>hms <span class="classifier-delimiter">:</span> <span class="classifier">bool, optional</span></dt>
<dd>Produce output in HH:MM:SS.S format instead of decimal degrees? (default: False)</dd>
<dt>precision <span class="classifier-delimiter">:</span> <span class="classifier">int, optional</span></dt>
<dd>Number of floating-point digits in output values</dd>
<dt>output <span class="classifier-delimiter">:</span> <span class="classifier">str, optional</span></dt>
<dd>Name of output file with results, if desired</dd>
<dt>verbose <span class="classifier-delimiter">:</span> <span class="classifier">bool</span></dt>
<dd>Print out full list of transformation results (default: False)</dd>
</dl>
</div>
<div class="section" id="returns">
<h2>RETURNS<a class="headerlink" href="#returns" title="Permalink to this headline">¶</a></h2>
<dl class="docutils">
<dt>ra <span class="classifier-delimiter">:</span> <span class="classifier">float</span></dt>
<dd>Right Ascension of pixel. If more than 1 input value, then it will be a
numpy array.</dd>
<dt>dec <span class="classifier-delimiter">:</span> <span class="classifier">float</span></dt>
<dd>Declination of pixel. If more than 1 input value, then it will be a
numpy array.</dd>
</dl>
</div>
<div class="section" id="notes">
<h2>NOTES<a class="headerlink" href="#notes" title="Permalink to this headline">¶</a></h2>
<p>This module performs a full distortion-corrected coordinate transformation
based on all WCS keywords and any recognized distortion keywords from the
input image header.</p>
</div>
<div class="section" id="usage">
<h2>Usage<a class="headerlink" href="#usage" title="Permalink to this headline">¶</a></h2>
<p>It can be called from within Python using the syntax:</p>
<div class="highlight-python"><div class="highlight"><pre><span class="gp">&gt;&gt;&gt; </span><span class="kn">from</span> <span class="nn">drizzlepac</span> <span class="kn">import</span> <span class="n">pixtosky</span>
<span class="gp">&gt;&gt;&gt; </span><span class="n">r</span><span class="p">,</span><span class="n">d</span> <span class="o">=</span> <span class="n">pixtosky</span><span class="o">.</span><span class="n">xy2rd</span><span class="p">(</span><span class="s">&quot;input_flt.fits[sci,1]&quot;</span><span class="p">,</span><span class="mi">100</span><span class="p">,</span><span class="mi">100</span><span class="p">)</span>
</pre></div>
</div>
</div>
<div class="section" id="examples">
<h2>EXAMPLES<a class="headerlink" href="#examples" title="Permalink to this headline">¶</a></h2>
<ol class="arabic">
<li><dl class="first docutils">
<dt>The following command will transform the position 256,256 into a</dt>
<dd><p class="first">position on the sky for the image &#8216;input_flt.fits[sci,1]&#8217; using:</p>
<div class="last highlight-python"><div class="highlight"><pre><span class="gp">&gt;&gt;&gt; </span><span class="kn">from</span> <span class="nn">drizzlepac</span> <span class="kn">import</span> <span class="n">pixtosky</span>
<span class="gp">&gt;&gt;&gt; </span><span class="n">r</span><span class="p">,</span><span class="n">d</span> <span class="o">=</span> <span class="n">pixtosky</span><span class="o">.</span><span class="n">xy2rd</span><span class="p">(</span><span class="s">&quot;input_file_flt.fits[sci,1]&quot;</span><span class="p">,</span> <span class="mi">256</span><span class="p">,</span><span class="mi">256</span><span class="p">)</span>
</pre></div>
</div>
</dd>
</dl>
</li>
<li><dl class="first docutils">
<dt>The set of X,Y positions from &#8216;input_flt.fits[sci,1]&#8217; stored as</dt>
<dd><p class="first">the 3rd and 4th columns from the ASCII file &#8216;xy_sci1.dat&#8217;
will be transformed and written out to &#8216;radec_sci1.dat&#8217; using:</p>
<div class="last highlight-python"><div class="highlight"><pre><span class="gp">&gt;&gt;&gt; </span><span class="kn">from</span> <span class="nn">drizzlepac</span> <span class="kn">import</span> <span class="n">pixtosky</span>
<span class="gp">&gt;&gt;&gt; </span><span class="n">r</span><span class="p">,</span><span class="n">d</span> <span class="o">=</span> <span class="n">pixtosky</span><span class="o">.</span><span class="n">xy2rd</span><span class="p">(</span><span class="s">&quot;input_flt.fits[sci,1]&quot;</span><span class="p">,</span> <span class="n">coords</span><span class="o">=</span><span class="s">&#39;xy_sci1.dat&#39;</span><span class="p">,</span>
<span class="go">    colnames=[&#39;c3&#39;,&#39;c4&#39;], output=&quot;radec_sci1.dat&quot;)</span>
</pre></div>
</div>
</dd>
</dl>
</li>
</ol>
</div>
<dl class="function">
<dt id="drizzlepac.pixtosky.xy2rd">
<tt class="descclassname">drizzlepac.pixtosky.</tt><tt class="descname">xy2rd</tt><big>(</big><em>input</em>, <em>x=None</em>, <em>y=None</em>, <em>coords=None</em>, <em>colnames=None</em>, <em>separator=None</em>, <em>hms=True</em>, <em>precision=6</em>, <em>output=None</em>, <em>verbose=True</em><big>)</big><a class="headerlink" href="#drizzlepac.pixtosky.xy2rd" title="Permalink to this definition">¶</a></dt>
<dd><p>Primary interface to perform coordinate transformations from
pixel to sky coordinates using STWCS and full distortion models
read from the input image header.</p>
</dd></dl>

</div>


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