% @(#)testb1ccd.hlq 17.1.1.1 (ESO-SDAG) 01/25/02 17:49:45 %++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ %.COPYRIGHT (c) 1994 European Southern Observatory %.IDENT testb1ccd.hlq %.AUTHOR RHW, SDAG/ESO %.KEYWORDS MIDAS, ccd package, bias, testing %.PURPOSE On-line help file for the command: TESTB1/CCD %.VERSION 940620 RHW created %.VERSION 950210 RHW txt output eliminated; printed info reduced %--------------------------------------------------------------------- \se SECTION./CCD \es\co TESTB1/CCD 20-Jun-1994 RHW \oc\su TEST1/CCD in_cat [out_id] [meth] [option] Combine bias frames stored in a catalogue and display it \us\pu Purpose: Combine bias frames stored in a catalogue and display it \up\sy Syntax: TESTB1/CCD in_cat [out_id] [meth] [option] \ys\pa in_cat = input (with the extension .cat) catalogue of frames to be combined; no default \ap\pa out_id = output identifier for the output of the test prodedure. All output (i.e. frames, listings and plots) will start with this identifier. Default is BIAS. \ap\pa meth = combining method for creation of the master bias frame. Possible methods are: sum - simple sum of all input input images;\\ ave(rage) - combined by averaging;\\ median - combining by medianing each pixel;\\ min(reject) - reject the min value from the average;\\ max(reject) - reject the max value from the average;\\ minmax(reject) - reject min and max from the average;\\ sig(clip) - sigma clipping to each pixel;\\ avsig(clip) - sigma clipping with minmax rejection;\\ Default is the average sigma cliping method. In case a clipping algoritms is used the CCD keyword BS_CLP will be read to get the clipping factors. \ap\pa option = Option to enable overwriting of existing combined bias frame. Default is `N' (i.e. no overwrite). \ap\no Note: This command is the first or a series of test commands on bias frames: B1 to B5. The complete test is executed by the command TESTBA/CCD. \\ To avoid unnecessary computations the command checks for the presence of the combined bias. If the overwrite option `Y' is used the existing combined bias output frame will be overwritten. \\ For more details about the various combining methods, please refer to the CCD Chapter in Volume B of the ESO-MIDAS Users' Guide. \on\op Output: The command will stored the outputs in a number of ascii and postscript files (preceding by the identification string out_id):\\ `out_id'.bdf: the combined bias frame;\\ `out_id'.ps: postscript file with an image of the combined bias frame;\\ \\ Keywords BIASMEAN, BIASSIGM are filled with the mean bias and its standard deviation. \po\see See also: TESTBA/CCD, SET/CCD, SHOW/CCD, COMBINE/CCD, AVERAGE/ROW, AVERAGE/COLUMN, FILTER/MEDIAN, Ch. 3 in Vol. 2 of the Users Guide. \ees\exs Examples: \ex TESTB1/CCD bs_cat.cat BS median Run the test procedure on the frame in the catalogue bs_cat. Combine the frame in a master frame BS using a median filter. All output will start with the identifier BS. \xe \sxe