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object --+
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WCSBase --+
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pywcs.WCS --+
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SIP
An extended version of WCS that supports Simple (or Spitzer) Imaging Polynomial (SIP) distortion coefficients. In addition to all of the functionality of regular WCS objects, SIP objects also provide pix2foc and foc2pix to correct/apply the SIP distortion.
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| a new object with type S, a subtype of T |
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| world |
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| pixel |
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Inherited from |
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| Properties | |
| string |
alt Character code for alternate coordinate descriptions. (Inherited from pywcs.WCSBase) |
| array[2][2] of double |
cdCDi_ja linear transformation matrix.
(Inherited from pywcs.WCSBase)
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| array[naxis] of double |
cdelt Coordinate increments ( CDELTia) for each coord axis.
(Inherited from pywcs.WCSBase)
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| list of strings |
cname A list of the coordinate axis names, CNAMEia.
(Inherited from pywcs.WCSBase)
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| array[naxis] of int |
colax An array recording the column numbers for each axis in a pixel list. (Inherited from pywcs.WCSBase) |
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colnum Where the coordinate representation is associated with an image-array column in a FITS binary table, this variable may be used to record the relevant column number. (Inherited from pywcs.WCSBase) |
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| array[naxis] of double |
crder The random error in each coordinate axis, CRDERia.
(Inherited from pywcs.WCSBase)
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| array[2][2] of double |
crotaCROTAia keyvalues for each coordinate axis.
(Inherited from pywcs.WCSBase)
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| array[naxis] of double |
crpix Coordinate reference pixels ( CRPIXja) for each pixel
axis.
(Inherited from pywcs.WCSBase)
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| array[naxis] of double |
crval Coordinate reference values ( CRVALia) for each
coordinate axis.
(Inherited from pywcs.WCSBase)
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| array[naxis] of double |
csyer The systematic error in the coordinate value axes, CSYERia.
(Inherited from pywcs.WCSBase)
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| list of strings |
ctype List of CTYPEia keyvalues.
(Inherited from pywcs.WCSBase)
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| int |
cubeface Index into the pixcrd (pixel coordinate) array for the
CUBEFACE axis.
(Inherited from pywcs.WCSBase)
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| list of strings |
cunit List of CUNITia keyvalues which define the units of
measurement of the CRVALia, CDELTia and
CDi_ja keywords.
(Inherited from pywcs.WCSBase)
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| string |
dateavg Representative mid-point of the date of observation in ISO format, yyyy-mm-ddThh:mm:ss.
(Inherited from pywcs.WCSBase)
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| string |
dateobs Start of the date of observation in ISO format, yyyy-mm-ddThh:mm:ss.
(Inherited from pywcs.WCSBase)
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| float |
equinox The equinox associated with dynamical equatorial or ecliptic coordinate systems, EQUINOXa (or EPOCH in
older headers).
(Inherited from pywcs.WCSBase)
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| int |
lat The index into the world coordinate array containing latitude values. (Inherited from pywcs.WCSBase) |
| float |
latpole The native latitude of the celestial pole, LATPOLEa
(deg).
(Inherited from pywcs.WCSBase)
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| int |
lng The index into the world coordinate array containing longitude values. (Inherited from pywcs.WCSBase) |
| float |
lonpole The native longitude of the celestial pole, LONPOLEa
(deg).
(Inherited from pywcs.WCSBase)
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| float |
mjdavg Modified Julian Date (MJD = JD - 2400000.5), MJD-AVG,
corresponding to DATE-AVG.
(Inherited from pywcs.WCSBase)
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| float |
mjdobs Modified Julian Date (MJD = JD - 2400000.5), MJD-OBS,
corresponding to DATE-OBS.
(Inherited from pywcs.WCSBase)
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| string |
name The name given to the coordinate representation WCSNAMEa.
(Inherited from pywcs.WCSBase)
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| int |
naxis The number of axes (pixel and coordinate), given by the NAXIS or WCSAXESa keyvalues.
(Inherited from pywcs.WCSBase)
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| array[3] of double |
obsgeo Location of the observer in a standard terrestrial reference frame, OBSGEO-X, OBSGEO-Y, OBSGEO-Z
(in metres).
(Inherited from pywcs.WCSBase)
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| array[2][2] of double |
pc The PCi_ja (pixel coordinate) transformation matrix.
(Inherited from pywcs.WCSBase)
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| list of tuples |
psPSi_ma keywords for each i and m.
(Inherited from pywcs.WCSBase)
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| list of tuples |
pvPVi_ma keywords for each i and m.
(Inherited from pywcs.WCSBase)
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| string |
radesys The equatorial or ecliptic coordinate system type, RADESYSa.
(Inherited from pywcs.WCSBase)
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| float |
restfrq Rest frequency (Hz) from RESTFRQa.
(Inherited from pywcs.WCSBase)
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| float |
restwav Rest wavelength (m) from RESTWAVa.
(Inherited from pywcs.WCSBase)
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| int |
spec The index containing the spectral axis values. (Inherited from pywcs.WCSBase) |
| string |
specsys Spectral reference frame (standard of rest), SPECSYSa
(Inherited from pywcs.WCSBase)
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| string |
ssysobs The actual spectral reference frame in which there is no differential variation in the spectral coordinate across the field-of-view, SSYSOBSa.
(Inherited from pywcs.WCSBase)
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| string |
ssyssrc The spectral reference frame (standard of rest) in which the redshift was measured, SSYSSRCa.
(Inherited from pywcs.WCSBase)
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| float |
velangl The angle in degrees that should be used to decompose an observed velocity into radial and transverse components. (Inherited from pywcs.WCSBase) |
| float |
velosys The relative radial velocity (m/s) between the observer and the selected standard of rest in the direction of the celestial reference coordinate, VELOSYSa.
(Inherited from pywcs.WCSBase)
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| float |
zsource The redshift, ZSOURCEa, of the source.
(Inherited from pywcs.WCSBase)
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Inherited from |
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| Method Details |
x.__init__(...) initializes x; see x.__class__.__doc__ for signature
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Convert focal plane coordinates to pixel coordinates. Pixel coordinates are zero-based.
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Convert pixel coordinates to focal plane coordinates. Pixel coordinates are zero-based.
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