wcs-xy2rd(1)

wcs-xy2rd1

Convert lists of pixel from (x,y) to (ra,dec) positions.

Usage

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

Releases

Unchanged in 5 releases since Debian 9 (Stretch).

  1. 9–13

Author

The Astrometry.net team. Principal investigators are David W. Hogg (NYU) and Dustin Lang (CMU).

From astrometry.net 0.97+dfsg-2 in Debian 13 (Trixie). Parsed by carta from the page's man source.