** How to Apply the Distortion Map File [#k5291a01] The distotion map can be simply applied by IRAF ccsetwcs command; #pre{{ ccsetwcs (image file) (s11a-band.db) (s11a-band.coo) }} . ** How the Files are Made [#s04301e7] The distortion map is measured using the data of galactic plane, where the number density of stars are high.~ The coordinates of the detected stars are matched with those in the 2MASS catalog (which are written in s11a-band.coo), and the distortion map (s11a-band.db) is produced by IRAF ccmap command with 5th order polynominal; #pre{{ ccmap s11a-band.coo s11a-band.db lngunit="degree" latunits="degrees" projection="tnx" xxorder=6 xyorder=6 yxorder=6 yyorder=6 maxiter=3 reject=4 }} .