astropy.wcs began life as pywcs. Earlier version numbers refer to
pywcs Version 1.11
- Updated to wcslib version 4.8, which gives much more detailed error
- Added functions get_pc() and get_cdelt(). These provide a way to
always get the canonical representation of the linear transformation
matrix, whether the header specified it in PC, CD or CROTA form.
- Long-running process will now release the Python GIL to better
support Python multithreading.
- The dimensions of the cd and
pc matrices were always returned as 2x2. They
now are sized according to naxis.
- Supports Python 3.x
- Builds on Microsoft Windows without severely patching wcslib.
- Lots of new unit tests
- pywcs will now run without pyfits, though the SIP and distortion
lookup table functionality is unavailable.
- Setting cunit will now verify that the values
are valid unit strings.
pywcs Version 1.10
- Adds a UnitConversion class, which gives access to wcslib’s unit
conversion functionality. Given two convertible unit strings, pywcs
can convert arrays of values from one to the other.
- Now uses wcslib 4.7
- Changes to some wcs values would not always calculate secondary values.
pywcs Version 1.9
Support binary image arrays and pixel list format WCS by presenting
a way to call wcslib’s wcsbth()
Updated underlying wcslib to version 4.5, which fixes the following:
- Fixed the interpretation of VELREF when translating
AIPS-convention spectral types. Such translation is now handled
by a new special- purpose function, spcaips(). The wcsprm
struct has been augmented with an entry for velref which is
filled by wcspih() and wcsbth(). Previously, selection by
VELREF of the radio or optical velocity convention for type VELO
was not properly handled.
- The pc member is now available with a default
raw Wcsprm object.
- Make properties that return arrays read-only, since modifying a
(mutable) array could result in secondary values not being
recomputed based on those changes.
- float properties can now be set using int values
pywcs Version 1.3a1
Earlier versions of pywcs had two versions of every conversion method:
X(...) -- treats the origin of pixel coordinates at (0, 0)
X_fits(...) -- treats the origin of pixel coordinates at (1, 1)
From version 1.3 onwards, there is only one method for each
conversion, with an ‘origin’ argument:
- 0: places the origin at (0, 0), which is the C/Numpy convention.
- 1: places the origin at (1, 1), which is the Fortran/FITS