% @(#)normalmos.hlq 1.2 (ESO-DMD) 2/14/94 14:21:16 %++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ %.COPYRIGHT (c) 1994 European Southern Observatory %.IDENT normalmos.hlq %.AUTHOR PB, DMD/ESO %.KEYWORDS MIDAS, help files, NORMALIZE/MOS %.PURPOSE On-line help file for the command: NORMALIZE/MOS %.VERSION 1.0 14-FEB-1994 : Creation, PB %---------------------------------------------------------------- \se SECTION./MOS \es\co NORMALIZE/MOS 19-AUG-1993 OS \oc\su NORMALIZE/MOS [ff] [table] [normff] [order] [method] Normalize MOS flat-field frame \us\pu Purpose: Normalize MOS flat-field frame \up\sy Syntax: NORM/MOS [ff] [table] [normff] [order] [method] \ys\pa ff = flat field image Session keyword: FLAT Default: flat table = Input table with slitlet positions Session keyword: MOS Default: mos normff = Output image Session keyword: NORMFLAT Default: normflat order = order of fit, or width of median filter Session keyword: FFORD Default: 3 method = smoothing method (median or polynomial) Session keyword: NORMMET Default: poly \ap\sa See also: FLAT/MOS \as\no Note: This command will fit a polynomial of order ORDER to the flat FF (resp. smooth FF with a median filter of width ORDER), and divide the flat by its smooth version, thereby creating the normalized flat NORMFF. This normalized flat should now only show the high-frequency pixel-to-pixel variations of the CCD sensitivity. \on\exs Examples: \ex NORMA/MOS flat mos normflat 2 poly Takes flat.bdf and fits within the limits given by mos.tbl a 2nd order polynomials to the spectral characteristics of the intensity. Divides flat.bdf by these fits and stores the results in normflat.bdf. NORMA/MOS ff ? normff 5 median Takes ff.bdf and smooths it with a median filter of 5 pixels width within the limits given by the table stored in keyword MOS. Divides ff.bdf by the smoothed frame and stores the results in normflat.bdf. \xe \sxe