wcs-pv2sip(1)

wcs-pv2sip1

Convert tpv wcs headers to sip distortion headers

Usage

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)

Releases

Unchanged in 5 releases since Debian 9 (Stretch).

  1. 9–13

Author

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

From astrometry.net 0.97+dfsg-2 in Debian 13 (Trixie). Parsed by carta from the page's man source.