% @(#)responlong.hlq 17.1.1.1 (ESO-IPG) 01/25/02 17:53:26 %++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ %.COPYRIGHT (c) 1993 European Southern Observatory %.IDENT responlong.hlq %.AUTHOR 23-MAR-93, IPG/ESO %.KEYWORDS MIDAS, help files, %.PURPOSE On-line help file for the command: RESPONSE/LONG %.VERSION 1.0 PB : Creation, 23-MAR-93 %---------------------------------------------------------------- \se SECTION./LONG \es\co RESPONSE/LONG PB 23-MAR-93 \oc\su RESPONSE/LONG [plot] [fit] [deg] [smo] [table] [image] [visu] Converts the response correction from table to image format. \us\pu Purpose: The response correction table resulting from INTEGRATE/LONG (and optionally edited by EDIT/FLUX) is converted to an image in wavelength-ratio or wavelength-color space. The interpolation is performed by polynomial or smoothing splines. \up\sy Syntax: RESPONSE/LONG [plot] [fit] [deg] [smo] [table] [image] [visu] \ys\pa plot = Type of plot: RATIO or MAGNITUDE \\ Session keyword: PLOTYP; default : RATIO \ap\pa fit = Type of fit (POLY or SPLINE). \\ Session keyword: FITYP; default : POLY \ap\pa deg = Degree of fit. \\ Session keyword: FITD; default : 3 \ap\pa smooth = Smoothing factor (used only if fit=SPLINE) \\ Session keyword : SMOOTH; default : 0. \ap\pa table = Response table, as supplied by INTEGRATE/LONG \\ Session keyword: RESPTAB; default : resp.tbl \ap\pa image = Output response image. \\ Session keyword: RESPONSE; default : response.bdf \ap\pa visu = Visualisation option: YES or NO \\ Session keyword: RESPLOT; default : YES \ap\sa See also: INTEGRATE/LONG, PLOT/RESPONSE, PLOT/FLUX, EXTINCTION/LONG,\\ EDIT/FLUX, CALIBRATE/FLUX \as\no Note: None. \on\exs Examples: \ex RESPONSE/LONG \xe \sxe