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+.. _updatewcs:
+
+**************************************
+UPDATEWCS
+**************************************
+UPDATEWCS applies corrections to the WCS of a science file
+and adds reference information as header keywords and fits
+file extensions so that a science file contains all necessary
+information to represent astrometrically precise positions.
+The order in which the corrections are applied is important
+and is as follows:
+
+- Detector to Image Correction
+
+- Apply Time dependent distortion (if applciable)
+
+- Recomputing the basic WCS
+
+- Apply Velocity Aberration Correction
+
+- Apply polynomial distortion through the SIP coefficients
+
+- Apply non-polynomial distortion
+
+Mathematicall the entire transformation from detector to sky
+coordinates is described by:
+
+.. math:: (x',y') &= DET2IM(x,y)
+
+.. math:: \binom{u'}{v'} &= \binom{x' - CRPIX1}{y' - CRPIX2}
+
+.. math:: \left( \begin{array}{ll}
+ \alpha \\
+ \delta \\
+ \end{array} \right) &=
+ \left( \begin{array}{ll}
+ CRVAL1 \\
+ CRVAL2\\
+ \end{array} \right) +
+ \left( \begin{array}{cc}
+ CD11 & CD12 \\
+ CD21 & CD22\\
+ \end{array} \right)
+ \left( \begin{array}{ll}
+ u' + f(u',v') + LT_x(x',y') \\
+ v' + g(u',v') + LT_y(x',y') \\
+ \end{array} \right)
+
+where f(u',v') and g(u',v') represent the polynomial distortion correction specified as
+
+.. math:: f(u',v') = \sum_{p+q=2}^{AORDER} A_{pq} {u'}^{p} {v'}^{q}
+ \\
+ g(u',v') = \sum_{p+q=2}^{BORDER} B_{pq} {u'}^{p} {v'}^{q}
+
+
+where
+
+* x', y' are the initial coordinates x,y with the 68th column correction applied through the DET2IM convention
+* u',v' are the DET2IM-corrected coordinates relative to CRPIX1,CRPIX2
+* LT<sub>x</sub>, LT<sub>y</sub> is the residual distortion in the lookup tables written to the header using the Paper IV lookup table convention
+* A, B are the SIP coefficients specified using the SIP convention
+
+.. toctree::
+ :maxdepth: 2
+
+ updatewcs_ui
+ apply_corrections
+ wcs_corrections \ No newline at end of file