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authordencheva <dencheva@stsci.edu>2012-10-31 15:30:13 -0400
committerdencheva <dencheva@stsci.edu>2012-10-31 15:30:13 -0400
commit4be66866b819e49c0ce23e40673879106cf6f5ab (patch)
tree9908c0ab74b63acfc7d4499052e18146530fee46 /doc/npol_tsr/source/index.rst
parent79824b1d42db580dc1473504488599945a2c7b48 (diff)
downloadstwcs_hcf-4be66866b819e49c0ce23e40673879106cf6f5ab.tar.gz
Added NPOL TSR
git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/stwcs@20138 fe389314-cf27-0410-b35b-8c050e845b92
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@@ -6,6 +6,19 @@ TSR 2012-03: NPOL Reference File
NPOL Reference File TSR
=======================
+.. abstract::
+ :author: Nadezhda Dencheva, Warren Hack
+ :date: 12 Oct 2010
+
+ The HST pipeline originally used two types of reference files to correct for distortion:
+ ``IDCTAB`` files which contain the coefficients for a polynomial correction and
+ ``DGEO`` files which are images with the residual distortion. A new format for the residual
+ distortion, called ``NPOL`` files (extension ``_npl.fits``), is presented in this document.
+ The conversion from ``DGEO`` files to ``NPOL`` files is described and an example of the format is given
+ using ACS/WFC F606W filter. Tests of the conversion procedure show that the
+ differences between the ``DGEO`` files and ``NPOL`` files are of the order of :math:`10^{-4}`
+ pixels.
+
Contents:
.. toctree::