---
name: "wcsremap"
section: "1"
platform: "linux"
package: "wcstools"
version: "3.9.7-1.1+b1"
release: "Debian 13 (Trixie)"
platforms: ["linux"]
url: "https://new.carta.tech/wcsremap"
---

# wcsremap(1)

AME

## NAME

wcsremap - AME

## SYNOPSIS

**remap** \[*-v*\]\[*-f WCSfile*\]\[*-a rot*\]\[\[*-b*\]\[*-j*\] *ra dec*\]\[*-i bits*\]\[*-l num*\] *file1.fit file2.fit* ... *filen.fit*

## DESCRIPTION

Remap FITS or IRAF images into single FITS image using WCS

-

  or : remap \[-v\]\[-f WCSfile\]\[-a rot\]\[\[-b\]\[-j\] ra dec\]\[-i bits\]\[-l num\] @filelist **-a**: Output rotation angle in degrees (default 0) **-b** ra dec: Output center in B1950 (FK4) RA and Dec **-e** long lat: Output center in ecliptic longitude and latitude **-f** file: Use WCS from this file as output WCS **-g** long lat: Output center in galactic longitude and latitude **-i** num: Number of bits per output pixel (default is input) **-j** ra dec: center in J2000 (FK5) RA and Dec **-l** num: Log every num rows of output image **-m** mode: c closest pixel (more to come) **-n** num: integer pixel value for blank pixel **-o** name: Name for output image **-p** secpix: Output plate scale in arcsec/pixel (default =input) **-s**: Set BZERO and BSCALE in output file from input file **-t**: Number of samples per linear output pixel **-u**: Delete distortion keywords from output file **-v**: Verbose **-w** type: Output WCS type (input is default) **-x** x y: Output image reference X and Y coordinates (default is center) **-y** nx ny: Output image dimensions (default is first input image)