| filename |
Name of FITS or IRAF image file. This must be present.
|
| -a rotation angle
| Output WCS rotation angle in degrees. The defauklt is to use the
same rotation angle as the input image.
|
| -b RA Dec |
Output center right ascension and declination in degrees or
sexigesimal in B1950 (FK4). Sexigesimal coordinates are
hours:minutes:seconds degrees:minutes:seconds.
The default is to use the input center, using the values of the
RA, DEC, and EPOCH keywords if there are
no standard WCS keywords in the image header.
|
| -e long lat |
Output center in ecliptic longitude and latitude in degrees.
|
| -f FITS filename |
Use WCS from the header of this file.
Other command line arguments can be used to override specific parameters.
(Added in WCSTools 3.4.2)
|
| -g long lat |
Output center in galactic longitude and latitude in degrees.
|
| -i number |
Bits per pixel in output image as FITS BITPIX values; i.e. -64 and -32
are 8-byte and 4-byte floating point numbers, and 8, 16, and 32 are
1-byte, 2-byte, and 4-byte integers.
|
| -j RA Dec |
Output center right ascension and declination in degrees or
sexigesimal in J2000 (FK5). Sexigesimal coordinates are
hours:minutes:seconds degrees:minutes:seconds.
The default is to use the input center, using the values of the
RA, DEC, and EPOCH keywords if there are
no standard WCS keywords in the image header.
|
| -l number |
Log every number rows of input image
|
| -n number |
Integer pixel value for output pixels not set from input image.
The BLANK header keyword is set to this value.
(Added in WCSTools 3.4.2)
|
| -o [filename] |
Write output to the file filename. The default is to write
a file called remap.fits.
|
| -p plate scale |
Output plate scale in arcseconds per pixel. The default is to use
the values of the SECPIX or SECPIX1 and SECPIX2
keywords in the image header). The default is to use the same plate scale
as the input image WCS.
|
| -v |
print more information about processing
|
| -w projection code |
The WCS projection of the output image, such as TAN. This is the
last 3/8ths of the output CTYPE1 and CTYPE2 keyword
values. The default is to use the same projection type as the input image.
The first five characters of these keywords are set based on the coordinate
system:
RA--- and DEC-- for -b (B1950) or -j (J2000),
GLON- and GLAT- for -g (galactic), and
ELON- and ELAT- for -e (ecliptic).
|
| -x Xref Yref |
Pixel coordinates of the reference pixel used in the output WCS projection
The default is to translate the input reference pixel into the output system.
|
| -y Xdim Ydim |
horizontal and vertical dimensions of the output image. The default is
to use the same as the input image.
|
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