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WCS-PV2SIP(1) astrometry.net WCS-PV2SIP(1)

wcs-pv2sip - Convert TPV WCS headers to SIP distortion headers

wcs-pv2sip [options] input-wcs output-wcs

-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)

The Astrometry.net team. Principal investigators are David W. Hogg (NYU) and Dustin Lang (CMU).

http://astrometry.net
July 2015 0.56

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