% @(#)load_cali.hlq 17.1.1.1 (ESO-IPG) 01/25/02 17:50:37 %++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ %.COPYRIGHT (c) 1995 European Southern Observatory %.IDENT load_cali.hlq %.AUTHOR PB, IPG/ESO %.KEYWORDS MIDAS, help files, LOAD/CALIBRATION %.PURPOSE On-line help file for the command: LOAD/CALIBRATION %.VERSION 1.0 10-AUG-1995 : Creation, PB %---------------------------------------------------------------- \se SECTION./CALI \es\co LOAD/CALIBRATION 10-AUG-1995 PB \oc\su LOAD/CALIBRATION display wavelength calibration result \us\pu Purpose: Displays the extracted and rebinned wavelength calibration frame for verification of the regularity of the order by order dispersion relations. \up\sy Syntax: LOAD/CALIBRATION [input] [output] \ys\pa input = Input image. By default the wavelength calibration frame (Session keyword: WLC). \ap\pa output = Output image. Default: middummr.bdf \ap\no Note: 1) Display cuts are copied from the input image. The output image can be reloaded with new cuts for a better visualisation. \\ 2) The wavelength range should regularly increase from bottom to top on the displayed image. \\ 3) If necessary the regularity of the dispersion relations can be improved by using the option WLCOPT=2D fitting a bivariate polynomial to the dispersion relation. Once a satisfactory calibration has been obtained with the method WLCMTD=PAIR, ANGLE or GUESS and WLCOPT=1D, new coefficients for the 2D solution are given with the sequence: \\ SET/ECHELLE WLCOPT=2D WLCMTD=ORDER \\ IDENT/ECHELLE \\ \\ 4) Method WLCMTD=ORDER can also be used to recompute the dispersion coefficients for another tolerance value (Session keyword TOL). \\ \on\sa See also: LOAD/IDENT, PLOT/RESIDUAL, IDENT/ECHELLE, REBIN/ECHELLE, LOAD/CALIB, PLOT/CALIB, PLOT/IDENT \\ \as\exs Examples: \ex LOAD/CALIB \xe\sxe