.TH FIT-WCS "1" "July 2015" "0.56" "astrometry.net"
.SH NAME
fit-wcs \- Fit a transformation from x,y and matching RA,DEC coordinates
.SH SYNOPSIS
.B fit-wcs
[options] \fB-x\fR file \fB-r file\fR
.br
.B fit-wcs
[options] \fB-c\fR file
.SH DESCRIPTION
Given a list of x,y coordinates and matching RA,Dec coordinates,
fit a transformation and produce a WCS file
.SH OPTIONS
.TP
\fB\-x\fR \fIfile\fP
XYls input file
.TP
\fB\-X\fR \fIname\fP
X column name (default: FIELD_X)
.TP
\fB\-Y\fR \fIname\fP
Y column name (default: FIELD_Y)
.TP
\fB\-r\fR \fIfile\fP
RDls input file
.TP
\fB\-R\fR \fIname\fP
RA column name (default: INDEX_RA)
.TP
\fB\-D\fR \fIname\fP
Dec column name (default: INDEX_DEC)
.TP
\fB\-c\fR \fIfile\fP
Correspondences file
.TP
\fB\-o\fR \fIfile\fP
WCS output file
.TP
\fB\-s \fIsip\fP
SIP order (default is a WCS TAN solution, not SIP)
.TP
\fB\-W \fIwidth\fP
Image width (default: max X position; used for SIP)
.TP
\fB\-H \fIheight\fP
Image height (default: max Y position; used for SIP)
.TP
\fB\-C\fR
Set CRPIX to be the center of the field; SIP only
.TP
\fB\-v
Verbose
.SH AUTHOR
The Astrometry.net team. Principal investigators are David W. Hogg (NYU) and
Dustin Lang (CMU).
.SH SEE ALSO
http://astrometry.net