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<li><a class="reference internal" href="#">Appendix 2 - NPOLFILE Example</a><ul>
<li><a class="reference internal" href="#fits-file-extensions">FITS File Extensions</a></li>
<li><a class="reference internal" href="#primary-header">Primary Header</a></li>
<li><a class="reference internal" href="#data-extension-header">Data Extension Header</a></li>
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  <div class="section" id="appendix-2-npolfile-example">
<span id="appendix2"></span><h1>Appendix 2 - NPOLFILE Example<a class="headerlink" href="#appendix-2-npolfile-example" title="Permalink to this headline">¶</a></h1>
<p>The NPOLFILE reference file format includes a PRIMARY header describing what kind of
image should be corrected by this file, along with extensions containing the corrections
for each chip.</p>
<div class="section" id="fits-file-extensions">
<h2>FITS File Extensions<a class="headerlink" href="#fits-file-extensions" title="Permalink to this headline">¶</a></h2>
<p>A sample NPOLFILE applicable to ACS/WFC F475W images has the FITS extensions:</p>
<div class="highlight-python"><pre>Filename: /grp/hst/cdbs/jref/v971826aj_npl.fits
No.    Name         Type      Cards   Dimensions   Format
0    PRIMARY     PrimaryHDU      35   ()           int16
1    DX          ImageHDU       180   (65, 33)     float32
2    DY          ImageHDU       215   (65, 33)     float32
3    DX          ImageHDU       215   (65, 33)     float32
4    DY          ImageHDU       215   (65, 33)     float32</pre>
</div>
<p>The extensions with the name &#8216;DX&#8217; provide the corrections in X for each of the
ACS/WFC&#8217;s 2 chips, while the &#8216;DY&#8217; extensions provide the corrections in Y for each chip.</p>
</div>
<div class="section" id="primary-header">
<h2>Primary Header<a class="headerlink" href="#primary-header" title="Permalink to this headline">¶</a></h2>
<p>The PRIMARY header of this file only includes the minimum information necessary to describe
what exposures should be corrected by this reference file and how it was generated. A full
listing of the PRIMARY header includes:</p>
<div class="highlight-python"><pre>SIMPLE  =                    T / Fits standard
BITPIX  =                   16 / Bits per pixel
NAXIS   =                    0 / Number of axes
EXTEND  =                    T / File may contain extensions
ORIGIN  = 'NOAO-IRAF FITS Image Kernel July 2003' / FITS file originator
IRAF-TLM= '2011-09-09T13:24:40'
NEXTEND =                    4 / Number of standard extensions
DATE    = '2010-04-02T19:53:08'
FILENAME= 'v971826aj_npl.fits' / name of file
FILETYPE= 'DXY GRID'           / type of data found in data file
OBSTYPE = 'IMAGING '           / type of observation
TELESCOP= 'HST'                / telescope used to acquire data
INSTRUME= 'ACS   '             / identifier for instrument used to acquire data
DETECTOR= 'WFC'                / detector in use: WFC, HRC, or SBC
FILTER1 = 'F475W   '           / element selected from filter wheel 1
FILTER2 = 'CLEAR2L '           / element selected from filter wheel 2
USEAFTER= 'Mar 01 2002 00:00:00'
COMMENT = 'NPOL calibration file created by Ray A. Lucas 29 APR 2010'
DESCRIP = 'Residual geometric distortion file for use with astrodrizzle-------'
PEDIGREE= 'INFLIGHT 11/11/2002 11/11/2002'
HISTORY   Non-polynomial offset file generated from qbu16420j_dxy.fits
HISTORY   Only added to the flt.fits file and used in coordinate
HISTORY   transformations if the npol reference filename is specified in
HISTORY   the header.  The offsets are copied from the reference file into
HISTORY   two arrays for each chip.  Each array is stored as a 65x33 pixel
HISTORY   image that gets interpolated up to the full chip size. Two new
HISTORY   extensions for each chip are also appended to the flt file
HISTORY   (WCSDVARR).
HISTORY qbu16420j_npl.fits renamed to v9615069j_npl.fits on Sep 6 2011
HISTORY v9615069j_npl.fits renamed to v971826aj_npl.fits on Sep 7 2011</pre>
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<div class="section" id="data-extension-header">
<h2>Data Extension Header<a class="headerlink" href="#data-extension-header" title="Permalink to this headline">¶</a></h2>
<p>Each ACS/WFC chip has a shape of 4096 x 2048 pixels,
yet the data arrays in this specific reference file only have 65x33 values.
Each data extension (&#8216;DX&#8217; and &#8216;DY&#8217;) contains only those keywords necessary to
properly interpolate the sub-sampled values from the arrays to apply to each individual
pixel in the full ACS/WFC exposure. The full header for the [&#8216;DX&#8217;,1] extension contains:</p>
<div class="highlight-python"><pre>XTENSION= 'IMAGE   '           / Image extension
BITPIX  =                  -32 / Bits per pixel
NAXIS   =                    2 / Number of axes
NAXIS1  =                   65 / Axis length
NAXIS2  =                   33 / Axis length
PCOUNT  =                    0 / No 'random' parameters
GCOUNT  =                    1 / Only one group
EXTNAME = 'DX      '           / Extension name
EXTVER  =                    1 / Extension version
ORIGIN  = 'NOAO-IRAF FITS Image Kernel July 2003' / FITS file originator
INHERIT =                    F / Inherits global header
DATE    = '2004-04-28T16:44:21'
IRAF-TLM= '16:42:00 (30/11/2006)'
WCSDIM  =                    2
LTM1_1  =                   1.
LTM2_2  =                   1.
WAT0_001= 'system=physical'
WAT1_001= 'wtype=linear'
WAT2_001= 'wtype=linear'
CCDCHIP =                    2 / CCDCHIP from full size dgeo file
LTV1    =                    0
LTV2    =                    0
ONAXIS1 =                 4096 / NAXIS1 of full size dgeo file
ONAXIS2 =                 2048 / NAXIS2 of full size dgeo file
CDELT1  =                   64 / Coordinate increment along axis
CDELT2  =                   64 / Coordinate increment along axis</pre>
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