Man page - wcs-pv2sip(1)
Packages contains this manual
- fits-flip-endian(1)
- an-pnmtofits(1)
- wcs-rd2xy(1)
- tabsort(1)
- plot-constellations(1)
- solve-field(1)
- an-fitstopnm(1)
- wcsinfo(1)
- fits-guess-scale(1)
- query-starkd(1)
- wcs-match(1)
- wcs-to-tan(1)
- fitsgetext(1)
- fit-wcs(1)
- wcs-xy2rd(1)
- astrometry-engine(1)
- get-wcs(1)
- subtable(1)
- fits-column-merge(1)
- hpsplit(1)
- image2xy(1)
- coadd(1)
- wcs-pv2sip(1)
- wcs-grab(1)
- plotxy(1)
- downsample-fits(1)
- build-astrometry-index(1)
- pad-file(1)
- get-healpix(1)
- plotquad(1)
- new-wcs(1)
- wcs-resample(1)
apt-get install astrometry.net
Manual
WCS-PV2SIP
NAMESYNOPSIS
OPTIONS
AUTHOR
SEE ALSO
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)
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-e ext |
FITS HDU number to read WCS from (default 0 = primary) |
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-S |
Do NOT do the wcs_shift thing |
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-s |
Treat input as Scamp .head file |
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-t |
Override the CTYPE* cards in the WCS header, and assume they are TAN. |
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-v |
+verboseness |
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-W int |
Set the IMAGEW in the output file |
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-H int |
Set the IMAGEH in the output file |
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-x num |
x-low (default: 1) |
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-y num |
y-low (default: 1) |
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-X num |
x-high (default: image width) |
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-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