.\" DO NOT MODIFY THIS FILE!  It was generated by help2man 1.49.3.
.TH WCSREMAP "1" "February 2024" "wcsremap EB_SOURCE" "User Commands"
.SH NAME
wcsremap \- AME
.SH SYNOPSIS
.B remap
[\fI\,-v\/\fR][\fI\,-f WCSfile\/\fR][\fI\,-a rot\/\fR][[\fI\,-b\/\fR][\fI\,-j\/\fR] \fI\,ra dec\/\fR][\fI\,-i bits\/\fR][\fI\,-l num\/\fR] \fI\,file1.fit file2.fit \/\fR... \fI\,filen.fit\/\fR
.SH DESCRIPTION
Remap FITS or IRAF images into single FITS image using WCS
.IP
or : remap [\-v][\-f WCSfile][\-a rot][[\-b][\-j] ra dec][\-i bits][\-l num] @filelist
\fB\-a\fR: Output rotation angle in degrees (default 0)
\fB\-b\fR ra dec: Output center in B1950 (FK4) RA and Dec
\fB\-e\fR long lat: Output center in ecliptic longitude and latitude
\fB\-f\fR file: Use WCS from this file as output WCS
\fB\-g\fR long lat: Output center in galactic longitude and latitude
\fB\-i\fR num: Number of bits per output pixel (default is input)
\fB\-j\fR ra dec: center in J2000 (FK5) RA and Dec
\fB\-l\fR num: Log every num rows of output image
\fB\-m\fR mode: c closest pixel (more to come)
\fB\-n\fR num: integer pixel value for blank pixel
\fB\-o\fR name: Name for output image
\fB\-p\fR secpix: Output plate scale in arcsec/pixel (default =input)
\fB\-s\fR: Set BZERO and BSCALE in output file from input file
\fB\-t\fR: Number of samples per linear output pixel
\fB\-u\fR: Delete distortion keywords from output file
\fB\-v\fR: Verbose
\fB\-w\fR type: Output WCS type (input is default)
\fB\-x\fR x y: Output image reference X and Y coordinates (default is center)
\fB\-y\fR nx ny: Output image dimensions (default is first input image)