Man page - wcs-xy2rd(1)
Packages contas this manual
- fitsgetext(1)
- fits-guess-scale(1)
- query-starkd(1)
- get-healpix(1)
- new-wcs(1)
- hpsplit(1)
- fits-flip-endian(1)
- fits-column-merge(1)
- plotxy(1)
- wcs-to-tan(1)
- get-wcs(1)
- wcs-grab(1)
- subtable(1)
- pad-file(1)
- downsample-fits(1)
- solve-field(1)
- wcs-resample(1)
- build-astrometry-index(1)
- an-fitstopnm(1)
- wcsinfo(1)
- plot-constellations(1)
- wcs-xy2rd(1)
- image2xy(1)
- wcs-rd2xy(1)
- wcs-pv2sip(1)
- wcs-match(1)
- plotquad(1)
- tabsort(1)
- fit-wcs(1)
- astrometry-engine(1)
- coadd(1)
- an-pnmtofits(1)
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Manual
| WCS-XY2RD(1) | astrometry.net | WCS-XY2RD(1) |
NAME
wcs-xy2rd - Convert lists of pixel from (x,y) to (RA,Dec) positions.
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
| July 2015 | 0.56 |