| Commit message (Collapse) | Author | Age | Files | Lines |
... | |
|
|
|
|
|
| |
This version of STWCS (0.9.1) provides support for headerlets based on 'Headerlet Design' wiki document, and includes TEAL interfaces for all public headerlet functions. It also moves the TEAL interface for 'updatewcs' from 'astrodither' to this package. The TEAL interaces have been included as a new 'gui' sub-package in order to keep them separate from the remainder of the package's functionality.
git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/stwcs@13910 fe389314-cf27-0410-b35b-8c050e845b92
|
|
|
|
|
|
| |
properly reflect that the distortion model is specific to each input image.
git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/stwcs@13698 fe389314-cf27-0410-b35b-8c050e845b92
|
|
|
|
|
|
| |
to also include header keywords from the reference file's primary header. This information will provide the user with the source of the calibration data.
git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/stwcs@13649 fe389314-cf27-0410-b35b-8c050e845b92
|
|
|
|
|
|
| |
'utils.extract_rootname', so that the same conventions can be used and to eliminate problems that generate values such as 'IDC_./n7n18501j'.
git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/stwcs@13647 fe389314-cf27-0410-b35b-8c050e845b92
|
|
|
|
|
|
| |
when the coefficients are shifted in subarray mode
git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/stwcs@13646 fe389314-cf27-0410-b35b-8c050e845b92
|
|
|
|
| |
git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/stwcs@13641 fe389314-cf27-0410-b35b-8c050e845b92
|
|
|
|
|
|
| |
by 8/11/2011 version of Headerlet Design document. The function 'compute_distname' was moved from __init__ to utils for use in other STWCS routines if necessary.
git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/stwcs@13640 fe389314-cf27-0410-b35b-8c050e845b92
|
|
|
|
|
|
| |
taken in subarray mode.
git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/stwcs@13637 fe389314-cf27-0410-b35b-8c050e845b92
|
|
|
|
|
|
| |
keywords to a science header which does not have any HISTORY keywords. This caused problems with data processed using the IMPHTTAB, as that code no longer reports the files used for the photometry keyword computation as HISTORY keywords.
git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/stwcs@13616 fe389314-cf27-0410-b35b-8c050e845b92
|
|
|
|
| |
git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/stwcs@13552 fe389314-cf27-0410-b35b-8c050e845b92
|
|
|
|
|
|
| |
this change - wcsname, wcskey, clobber.
git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/stwcs@13548 fe389314-cf27-0410-b35b-8c050e845b92
|
|
|
|
|
|
| |
in order to be able to repeatedly run updatewcs on files.
git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/stwcs@13545 fe389314-cf27-0410-b35b-8c050e845b92
|
|
|
|
| |
git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/stwcs@13539 fe389314-cf27-0410-b35b-8c050e845b92
|
|
|
|
|
|
| |
primary WCS. Not passing input parameter check now raises an Error. Not findong a wcskey raises a KeyError.
git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/stwcs@13537 fe389314-cf27-0410-b35b-8c050e845b92
|
|
|
|
| |
git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/stwcs@13516 fe389314-cf27-0410-b35b-8c050e845b92
|
|
to the setup_refactoring branch (however, coords, pysynphot, and pywcs are still being pulled from the astrolib setup_refactoring branch. Will have to do that separately then update the svn:externals)
git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/stwcs@13225 fe389314-cf27-0410-b35b-8c050e845b92
|