%++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ %.COPYRIGHT (c) 1994 European Southern Observatory %.IDENT flatmos.hlq %.AUTHOR SM/LSW %.KEYWORDS MIDAS, help files, FLAT/MOS %.PURPOSE On-line help file for the command: FLAT/MOS %.VERSION 1.0 04-AUG-1994 : Creation, SM %---------------------------------------------------------------- \se SECTION./MOS \es\co FLAT/MOS 20-SEP-1994 SM \oc\su FLAT/MOS [obj] objf [ff] [mos] [normff] [order] [method] normalize MOS flat-field frame and divide object by it \us\pu Purpose: Normalize MOS flat-field frame and divide object frame by it \up\sy Syntax: FLAT/MOS [obj] objf [ff] [mos] [normff] [order] [method] \ys\pa obj = object image Session keyword: OBJECT Default: none objf = flat-field corrected object image ff = FF image Session keyword: FLAT Default: flat mos = Input table with slitlet positions Session keyword: MOS Default: mos normff = normalized flat field 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: NORMAL/MOS \ap\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 FF by the fitted resp. smoothed image, thereby creating the normalized flat NORMFF. This normalized flat should now only show the high-frequency pixel-to-pixel variations of the CCD sensitivity. Then the object frame OBJ is divided through the normalized flat. OBJF holds the output of this action. \on\exs Examples: \ex FLAT/MOS object objf flat mos normflat 3 poly Fits a 3rd order polynomial to the spectral signature of flat.bdf and thereby normalizes it to normflat.bdf. It then divides object.bdf by normflat.bdf and stores the result in objf.bdf. \xe \sxe