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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

http://astrometry.net

Info

July 2015 0.56 astrometry.net