wcs-pv2sip - Man Page
Convert TPV WCS headers to SIP distortion headers
Synopsis
wcs-pv2sip [options] input-wcs output-wcs
Options
- -o order
SIP polynomial order to fit (default: 5)
- -e ext
FITS HDU number to read WCS from (default 0 = primary)
- -S
Do NOT do the wcs_shift thing
- -s
Treat input as Scamp .head file
- -t
Override the CTYPE* cards in the WCS header, and assume they are TAN.
- -v
+verboseness
- -W int
Set the IMAGEW in the output file
- -H int
Set the IMAGEH in the output file
- -x num
x-low (default: 1)
- -y num
y-low (default: 1)
- -X num
x-high (default: image width)
- -Y num
y-high (default: image width)
- -a size
Set the pixel values used to compute the distortion polynomials with (default: closest to 100 yielding whole number of steps)
Author
The Astrometry.net team. Principal investigators are David W. Hogg (NYU) and Dustin Lang (CMU).
See Also
Info
July 2015 0.56 astrometry.net