wcs-xy2rd
Convert lists of pixel from (x,y) to (RA,Dec) positions.
- Provided by: astrometry.net (Version: 0.89+dfsg-1)
- Report a bug
SYNOPSIS
wcs-xy2rd [options] -w file
OPTIONS
- -w file
- WCS input file
- -e extension
- FITS HDU number to read WCS from (default 0 = primary)
- -x pixel -y pixel
- Specify a single point to convert (result is printed to stdout)
- -t
- just use TAN projection, even if SIP extension exists.
- -L
- force WCSlib
- -T
- force WCStools
- -s
- print sexigesimal too
- -i file
- xyls input file
- -o file
- rdls output file
- -f index
- xyls field index (default: all)
- -X name
- X-column-name
- -Y name
- Y-column-name
- -v
- +verbose
AUTHOR
The Astrometry.net team. Principal investigators are David W. Hogg (NYU) and Dustin Lang (CMU).
SEE ALSO
http://astrometry.net