gh_mirror/jhunkeler/stwcs_hcf.git/hstwcs/dgeo.py, branch pre-astropy

Renamed hstwcs to udpatewcs

2009-04-29T12:13:55+00:00

git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/development/trunk/stwcs@7976 fe389314-cf27-0410-b35b-8c050e845b92

Changed imports of numpy (as np).

2009-03-26T15:26:59+00:00

Added d2imcorr parameter to top level updatewcs function.



git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/development/trunk/updatewcs@7803 fe389314-cf27-0410-b35b-8c050e845b92

Added code which populates the science file with information about detector to image correction - header keywords and a lookup table extension. Cleaned coed.

2009-03-17T20:35:57+00:00

git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/development/trunk/updatewcs@7770 fe389314-cf27-0410-b35b-8c050e845b92

Changed the name of the kw recording the dgeofile used for the lookup tables to DGEOEXT.

2009-03-17T13:50:03+00:00

git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/development/trunk/updatewcs@7766 fe389314-cf27-0410-b35b-8c050e845b92

had the wrong value assigned to crpix2

2009-03-11T15:51:22+00:00

git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/development/trunk/updatewcs@7737 fe389314-cf27-0410-b35b-8c050e845b92

The DGEO files were defined to be used after the IDC polynomial coefficients. To use them with SIP coefficients the first order IDC coefficients should be backed out of the DGEO data by multiplying with the inverse of the scaled cd matrix. The scaling of the cd matrix was done incorrectly - fixed in this revision.

2009-03-10T15:28:53+00:00

git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/development/trunk/updatewcs@7732 fe389314-cf27-0410-b35b-8c050e845b92

Renamed updatewcs to hstwcs

2008-12-22T14:07:16+00:00

git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/development/trunk/hstwcs@7406 fe389314-cf27-0410-b35b-8c050e845b92