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

NAME
       wcs-pv2sip - 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
       http://astrometry.net

0.56				   July	2015			 WCS-PV2SIP(1)

NAME | SYNOPSIS | OPTIONS | AUTHOR | SEE ALSO

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