I've assembled a list of links to bring some order to the many astrometery codes I have been using. Most of these routines were then used to build a series of demostrations scripts (SimIm0, SimIm1, ...). Most of the scripts listed above are easy to use and well-documented (both online help via "-- help" and webpage documents). To demonstarte their use I am composing a set of scripts that allow some user interaction at runtime. The basic steps are to (1) build a simulated image, (2) apply a coordinate transformation to the image, (3) intsall WCS header in each of the two images that yield uniform astrometry.
Most of the scripts listed above are easy to use and well-documented (both online help via "-- help" and webpage documents). The goal here is to create a terse but clear sequence of commands that demontsrate the path to a WCS-calibrated image. The commands should closely follow the links above. The links (mostly to Big_Code_Table entries) give usage details.
The primary purose of these exercises is is t demsonstrate that I can transform images and properly compensate for these changes in the final WCS of the header, I manually made a region file of fk5 positions to aid in the demmo. If the region file (named "Test0.reg") is present in the directory where we run the SimIm* scripts, then the positions are overplotted in the original and the transformed images. Here is the region file I use:
% cat Test0.reg # Region file format: DS9 version 4.1 # Filename: Modelwcs.fits global color=green dashlist=8 3 width=1 font="helvetica 10 normal roman" select=1 highlite=1 dash=0 fixed=0 edit=1 move=1 delete=1 include=1 source=1 fk5 circle(12:00:04.763,+32:30:58.14,15.606") # color=black font="helvetica 12 normal roman" text={12:00:04.763 +32:30:58.14} circle(11:59:57.291,+32:30:00.76,18.1465") # color=black font="helvetica 12 normal roman" text={11:59:57.291 +32:30:00.76}