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object --+
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WCSBase --+
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WCS
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| a new object with type S, a subtype of T |
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| dict |
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| bool |
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| bool |
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| bool |
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| dict |
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| dict |
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| world |
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| dict |
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| int |
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| int |
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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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Transforms world coordinates to pixel coordinates. pixel2world is a convenience wrapper around p2s. If intermediate values from the transform are needed, use the more complex p2s directly.
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Transforms world coordinates to pixel coordinates. world2pixel is a convenience wrapper around s2p. If intermediate values from the transform are needed, use the more complex s2p directly.
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