The following world coordinate system (WCS) driven image registration tasks have been added to the new IRAF V2.11 **
immatch**
package.

The tasks**
wregister**
and **
sregister**
use the reference and input image coordinate systems to compute a grid of matched pixel coordinates, use the matched grid to compute a coordinate mapping from the reference image to the input images, compute the output image pixel values by interpolating in the input image at the position of the mapped reference image pixels, and update the output image coordinate systems. **
wregister**
can register images with any valid coordinate system provided that the reference and input image have the same coordinate system, e.g., both images have J2000.0 equatorial systems. **
sregister**
can only register images with celestial coordinate systems, e.g., equatorial J2000.0 or galactic, but can register images with different celestial coordinates systems, e.g., register an image with an FK4 B1950.0 coordinate system to one with an FK5 J2000.0 coordinate system.

Matched coordinate grids or coordinate mappings can be computed without doing the actual image registration by calling the supporting tasks **
wcsxymatch**
/**
wcsmap**
in the case of **
wregister**
, or the **
skyxymatch**
/ **
skymap**
tasks in the case of **
sregister**
. These tasks can be used to examine the coordinate mappings interactively.

The tasks**
wcsmap**
/**
skymap**
, **
wregister**
/**
sregister**
are script tasks which call **
wcsxymatch**
/**
skyxymatch**
to compute the respective matched coordinate grids, **
geomap**
to compute the required geometric transformations, **
geotran**
to do the actual image registration, and **
wcscopy**
to update the image coordinate system.