print sky coordinates as B1950 (FK4) right ascension and declination
-cfilename
File with polynomial coefficients for conversion of image magnitudes
to catalog magnitudes. The numbers can be anywhere in the file with the
format keyword=value, where keyword can
be mag0, mcoeff0, mcoeff1, ... mcoeff4, and the assignments can
be anywhere within the file.
The file to be read can be produced by the
immatch program if the -q command
is used. The image magnitude is expected to be in the third column
unless the xy2sky-c argument is used to specify a column.
(added in WCSTools 3.0.1)
-d
Print RA and Dec output in degrees
-e
Print sky coordinates as ecliptic longitude and latitude in degrees
-fnumber
Number of face to use for 3-d projection
-g
Print sky coordinates as galactic longitude and latitude
-i
First column is star id; 2nd, 3rd are x,y position
-j
print sky coordinates as J2000 (FK5) right ascension and declination
-lnumber
Mode for output of LINEAR WCS coordinates:
1= append units from CUNITi to each coordinate
2= append units from CUNITi at end of coordinate string
-mnumber
Column for magnitude on input; this defaults to 3 if the -c
command is used.
(Added in WCSTools 3.0.1)
-nnumber
Number of decimal places in output RA seconds or decimal degrees
-or or d or s
Print only RA, Dec, or coordinate system
-qfractional year
Output equinox if not 2000 or 1950
-t
Tab table output
-v
print more information about process
-xnumber
Column for image X coordinate; image Y coordinate is in the following
column.
(Added in WCSTools 3.0.1)
-z
Use AIPS classic projections instead of WCSLIB
filename
Name of FITS or IRAF image file. This must be present.
@filename
Name of file containing list of sky coordinate pairs in first two columns.
(Lines with # in the first column are ignored.)
or
x y
Image coordinate X Y pair.
There may be any number of these up to the maximum Unix line length, but they
MUST follow the image file name argument.
[xy2sky Examples]