The uses all the images, specifically the SUMFILE, to determine the pole of the object. You provide the time that you want the pole's RA/Dec. You can also solve for the rotational speed (w).
It will create the file POLE.TXT and updates all the landmarks and maplets (due to a different polar alignment)
= Input =
/usr/local/bin/POLE 1996-12-18T12:28:28 y