fit-wcs - Man Page
Fit a transformation from x,y and matching RA,DEC coordinates
Synopsis
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
Info
July 2015 0.56 astrometry.net