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1. CL Script for creating daily dark files
... CL Script for creating daily dark files . ... Data . ... The latter will ensure that one will also retrieve the appropriate "weekly bias" and "weekly dark" reference files. ... The parameter file should look like this: (Where basedark means the reference weekly dark ) infiles = Input dark image(s) to be combined/normalized basedark = Name of baseline superdark file (biasfile = ) Name of reference bias file to be used (outfile = day_ dark .fits ) Name of output normalized ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/stis/design/software/analyzing/scripts/daydark -- 24.5 Кб -- 12.04.2016
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2. TUI:Scripts:Scripting Tutorial:Refinements
Adding a few refinements to the DISCals script makes a script worth adapting for your own uses. ... The exposure times and # of iterations are short so the demo runs quickly. def __init__(self, sr): Display the exposure status panel. # if True, run in debug-only mode (which doesn't DO anything, it just pretends) sr.debug = False expStatusWdg = ExposeStatusWdg( master = sr.master, instName = DIS , ) expStatusWdg.grid(row=0, column=0) # get the exposure model self.expModel = ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/35m_operations/TUI/Scripts/ScriptingTutorial/Refinements.html -- 6.6 Кб -- 05.09.2014
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3. Making a Fake Observation
... The Miriad task uvgen can be used to simulate a variety of observing modes. ... Simulating a telescope approximately, let alone in some detail, requires a good many parameters. uvgen takes an appreciable number of parameters and input files to describe the telescope, correlator and source. Fortunately keyword and set-up files for some common situations exist ( e.g. simulating the ATCA and VLA). ... For example, to load typical parameters for the ATCA, use miriad% source $MIRCAT/uvgen.def.atca . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/miriad/userguide/node56.html -- 12.7 Кб -- 10.04.2016
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4. Parameters
... Meta Index / Home Page This section documents the parameters recognized by this task (if any). ... string . ... yes|no . Yes' forces overwrite of colimchain output. astest . ... Yes' invokes asmooth to smooth the input images before they are supplied to colimplot . ... The maximum allowed value of the width of the smoothing gaussian is specified via this parameter. desiredsnr . ... The maximum desired signal-to-noise ratio of the output image can be specified via this parameter. nconvolvers . ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/colimchain/node4.html -- 18.1 Кб -- 02.07.2008
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5. ccd
... BIAS/CCD [in_fram] [out_fram] [bs_fram] . Correct the input frame for the bias offset using a bias frame . COMBINE/CCD exp [in_spec] [out_fram] . ... Do a correction of bad pixels in the input frame . FLAT/CCD [in_fram] [out_fram] [ff_fram] . Do a flat field correction of the input frame . FRCOR/CCD [in_spec] [out_frm] [xboxmn,xboxmx] [yboxmn,yboxmx] [clip] . ... Do a fringe correction of the input frame . ... Do an illumination correction of the input frame . INIT/CCD [name] . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol1/node145.html -- 6.8 Кб -- 23.02.1996
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