% @(#)normalflat.hlq 17.1.1.1 (ESO-IPG) 01/25/02 17:53:24 %++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ %.COPYRIGHT (c) 1993 European Southern Observatory %.IDENT normalflat.hlq %.AUTHOR 23-MAR-93, IPG/ESO %.KEYWORDS MIDAS, help files, %.PURPOSE On-line help file for the command: NORMALIZE/FLAT %.VERSION 1.0 PB : Creation, 23-MAR-93 %---------------------------------------------------------------- \se SECTION./FLAT \es\co NORMALIZE/FLAT PB 1-AUG-95 \oc\su NORMALIZE/FLAT in out [bias] [deg] [fit] [visu] Normalisation of flat-fields \us\pu Purpose: The flat-field is divided by its average shape, obtained by fitting a polynomial along the dispersion direction of an averaged flat-field. \up\sy Syntax: NORMALIZE/FLAT in out [bias] [deg] [fit] [visu] \ys\pa in = input image, consisting of a flat-field or a combination of flat-fields (resulting from COMBINE/LONG). \ap\pa out = Name of the output normalised flat-field. \ap\pa bias = bias image or constant to be subtracted prior to normalisation. \\ Session keyword: BIAS; default: 0 \ap\pa deg = Order of the polynomial. \\ Session keyword: FDEG; default: 2 \ap\pa fit = fitted 1D spectrum used for normalisation. \\ Session keyword: FFIT; default: middummf.bdf \ap\pa visu = Visualisation flag (YES/NO). If visu=YES, the central row of the flat field is plotted as well as the fitted function. \\ Session keyword: FVISU; default: YES \ap\sa See also: COMBINE/LONG, CONTINUUM/SPEC \as\no Note: 1) Session keywords relative to this command are displayed by SHOW/LONG D 2) Smoothing spline fitting can be performed with the command CONTINUUM/SPEC. \on\exs Examples: \ex NORMALIZE/FLAT flat ffnorm deg=3 visu=no \xe \sxe