.TH WCS-RD2XY "1" "July 2015" "0.56" "astrometry.net"
.SH NAME
wcs-rd2xy \- Convert lists of pixel from (RA,Dec) to (x,y) positions.
.SH SYNOPSIS
.B wcs-rd2xy
[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\-i\fR \fIfile\fR
rdls input file
.TP
\fB\-o\fR \fIfile\fR
xyls output file
.TP
\fB\-f\fR \fIindex\fR
rdls field index (default: all)
.TP
\fB\-R\fR \fIname\fR
RA column name
.TP
\fB\-D\fR \fIname\fR
DEC column name
.TP
\fB\-t\fR
Just use TAN projection, even if SIP extension exists
.TP
\fB\-L\fR
Force using WCSlib rather than Astrometry.net routines
.TP
\fB\-r\fR \fIra\fR \fB\-d\fR \fIra\fR
Specify a single point (in deg) to convert (printed to stdout)
.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