Man page - fit-wcs(1)
Packages contas this manual
- fitsgetext(1)
- fits-guess-scale(1)
- query-starkd(1)
- get-healpix(1)
- new-wcs(1)
- hpsplit(1)
- fits-flip-endian(1)
- fits-column-merge(1)
- plotxy(1)
- wcs-to-tan(1)
- get-wcs(1)
- wcs-grab(1)
- subtable(1)
- pad-file(1)
- downsample-fits(1)
- solve-field(1)
- wcs-resample(1)
- build-astrometry-index(1)
- an-fitstopnm(1)
- wcsinfo(1)
- plot-constellations(1)
- wcs-xy2rd(1)
- image2xy(1)
- wcs-rd2xy(1)
- wcs-pv2sip(1)
- wcs-match(1)
- plotquad(1)
- tabsort(1)
- fit-wcs(1)
- astrometry-engine(1)
- coadd(1)
- an-pnmtofits(1)
Package: astrometry.net
apt-get install astrometry.net
apt-get install astrometry.net
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Manual
| FIT-WCS(1) | astrometry.net | FIT-WCS(1) |
NAME
fit-wcs - Fit a transformation from x,y and matching RA,DEC coordinates
SYNOPSIS
fit-wcs [options] -x file -r file
fit-wcs [options] -c file
DESCRIPTION
Given a list of x,y coordinates and matching RA,Dec coordinates, fit a transformation and produce a WCS file
OPTIONS
- -x file
- XYls input file
- -X name
- X column name (default: FIELD_X)
- -Y name
- Y column name (default: FIELD_Y)
- -r file
- RDls input file
- -R name
- RA column name (default: INDEX_RA)
- -D name
- Dec column name (default: INDEX_DEC)
- -c file
- Correspondences file
- -o file
- WCS output file
- -s sip
- SIP order (default is a WCS TAN solution, not SIP)
- -W width
- Image width (default: max X position; used for SIP)
- -H height
- Image height (default: max Y position; used for SIP)
- -C
- Set CRPIX to be the center of the field; SIP only
- -v
- Verbose
AUTHOR
The Astrometry.net team. Principal investigators are David W. Hogg (NYU) and Dustin Lang (CMU).
SEE ALSO
http://astrometry.net
| July 2015 | 0.56 |