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author | dencheva <dencheva@stsci.edu> | 2012-10-31 15:34:51 -0400 |
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committer | dencheva <dencheva@stsci.edu> | 2012-10-31 15:34:51 -0400 |
commit | bfc0125dac0b0612cdff9b8239e8040f2bd287dc (patch) | |
tree | 10047b8636d8ac21dad1401c3fb222a59c32aa8a /doc | |
parent | 6e1dc6c7b62318dd3b3e3a024f79258b44c7873a (diff) | |
download | stwcs_hcf-bfc0125dac0b0612cdff9b8239e8040f2bd287dc.tar.gz |
more changes to npol tsr
git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/stwcs@20141 fe389314-cf27-0410-b35b-8c050e845b92
Diffstat (limited to 'doc')
-rw-r--r-- | doc/npol_tsr/source/npol.rst | 13 |
1 files changed, 0 insertions, 13 deletions
diff --git a/doc/npol_tsr/source/npol.rst b/doc/npol_tsr/source/npol.rst index 80145ae..a6809cd 100644 --- a/doc/npol_tsr/source/npol.rst +++ b/doc/npol_tsr/source/npol.rst @@ -4,19 +4,6 @@ NPOL Reference File =================== -.. 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. - Introduction ============ |