reidentify

    reference =                 Reference image
       images =                 Images to be reidentified
       answer = "yes"           Fit dispersion function interactively?
crval = Approximate coordinate (at reference pixel)
cdelt = Approximate dispersion
(interactive = "no") Interactive fitting?
(section = "middle line") Section to apply to two dimensional images
(newaps = yes) Reidentify apertures in images not in reference
(override = no) Override previous solutions?
(refit = yes) Refit coordinate function?\n
(trace = no) Trace reference image?
(step = "10") Step in lines/columns/bands for tracing an imag
(nsum = "10") Number of lines/columns/bands to sum
(shift = "0.") Shift to add to reference features (INDEF to se
(search = 0.) Search radius
(nlost = 0) Maximum number of features which may be lost\n
(cradius = 5.) Centering radius
(threshold = 0.) Feature threshold for centering
(addfeatures = no) Add features from a line list?
(coordlist = "/astro/users/ben/premap/calibration/idhenear.dat") User coordinate list
(match = -3.) Coordinate list matching limit
(maxfeatures = 100) Maximum number of features for automatic identi
(minsep = 2.) Minimum pixel separation\n
(database = "database") Database
(logfiles = "logfile") List of log files
(plotfile = "") Plot file for residuals
(verbose = no) Verbose output?
(graphics = "stdgraph") Graphics output device
(cursor = "") Graphics cursor input\n
(aidpars = "") Automatic identification algorithm parameters
(mode = "ql")

NOTE: It is generally a good idea to fit the dispersion function interactively so that you cna keep an eye on what's going on. Hence the parameter setting answer = yes If for some reason you want the fits to be done automatically without your intervention, then set answer = no and you will get what you deserve.