wcs-xy2rd -V (return code: 255)
wcs-xy2rd: invalid option -- '-'
This program is part of the Astrometry.net suite.
For details, visit http://astrometry.net.
Git URL https://github.com/dstndstn/astrometry.net
Revision 0.72, date Mon_Jul_10_14:37:28_2017_-0400.
Usage: wcs-xy2rd
-w <WCS input file>
[-e <extension>] FITS HDU number to read WCS from (default 0 = primary)
[-t]: just use TAN projection, even if SIP extension exists.
[-L]: force WCSlib
[-T]: force WCStools
[-s]: print sexigesimal too
-i <xyls input file>
-o <rdls output file>
[-f <xyls field index>] (default: all)
[-X <x-column-name> -Y <y-column-name>]
[-v]: +verbose
You can also specify a single point to convert (result is printed to stdout):
[-x <pixel>]
[-y <pixel>]
wcs-xy2rd --help (return code: 0)
wcs-xy2rd: invalid option -- '-'
This program is part of the Astrometry.net suite.
For details, visit http://astrometry.net.
Git URL https://github.com/dstndstn/astrometry.net
Revision 0.72, date Mon_Jul_10_14:37:28_2017_-0400.
Usage: wcs-xy2rd
-w <WCS input file>
[-e <extension>] FITS HDU number to read WCS from (default 0 = primary)
[-t]: just use TAN projection, even if SIP extension exists.
[-L]: force WCSlib
[-T]: force WCStools
[-s]: print sexigesimal too
-i <xyls input file>
-o <rdls output file>
[-f <xyls field index>] (default: all)
[-X <x-column-name> -Y <y-column-name>]
[-v]: +verbose
You can also specify a single point to convert (result is printed to stdout):
[-x <pixel>]
[-y <pixel>]