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FIT-WCS(1) |
astrometry.net |
FIT-WCS(1) |
fit-wcs - Fit a transformation from x,y and matching RA,DEC coordinates
fit-wcs [options] -x file -r file
fit-wcs [options] -c file
Given a list of x,y coordinates and matching RA,Dec coordinates, fit a
transformation and produce a WCS file
- -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
The Astrometry.net team. Principal investigators are David W. Hogg (NYU) and
Dustin Lang (CMU).
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