.TH WCS-XY2RD "1" "July 2015" "0.56" "astrometry.net"
.SH NAME
wcs-xy2rd \- Convert lists of pixel from (x,y) to (RA,Dec) positions.
.SH SYNOPSIS
.B wcs-xy2rd
[options] \fB\-w\fR \fIfile\fR
.SH OPTIONS
.TP
\fB\-w\fR \fIfile\fR
WCS input file
.TP
\fB\-e\fR \fIextension\fR
FITS HDU number to read WCS from (default 0 = primary)
.TP
\fB\-x \fIpixel\fR \fB\-y \fIpixel\fR
Specify a single point to convert (result is printed to stdout)
.TP
\fB\-t\fR
just use TAN projection, even if SIP extension exists.
.TP
\fB\-L\fR
force WCSlib
.TP
\fB\-T\fR
force WCStools
.TP
\fB\-s\fR
print sexigesimal too
.TP
\fB\-i\fR \fIfile\fR
xyls input file
.TP
\fB\-o\fR \fIfile\fR
rdls output file
.TP
\fB\-f \fIindex\fR
xyls field index (default: all)
.TP
\fB\-X \fIname\fR
X-column-name
.TP
\fB\-Y\fR \fIname\fR
Y-column-name
.TP
\fB\-v\fR
+verbose
.SH AUTHOR
The Astrometry.net team. Principal investigators are David W. Hogg (NYU) and
Dustin Lang (CMU).
.SH SEE ALSO
http://astrometry.net