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

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

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

-oorder
              SIP polynomial order to fit (default: 5)

       -eext 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

       -Wint Set the IMAGEW in the output file

       -Hint Set the IMAGEH in the output file

       -xnum x-low (default: 1)

       -ynum y-low (default: 1)

       -Xnum x-high (default: image width)

       -Ynum y-high (default: image width)

       -asize
              Set  the  pixel  values  used  to compute the distortion polynomials with (default: closest to 100
              yielding whole number of steps)

http://astrometry.net

0.56                                                July 2015                                      WCS-PV2SIP(1)

wcs-pv2sip [options] input-wcsoutput-wcs