![]() The subtraction itself, by a high-pass filter (in Take the output of oir1dCompressData and form spectrally dispersedįringes by subtraction of the two interferometic channels and MaskFile except that the y-dimension of each DATA array is 1. This will be a MIDI styleįITS binary table in exactly the same format as "inFiles" and Specified it defaults to an environmental variable specifiedĮxternally (typically in the vltisetup script): MaskFile: a MIDI style FITS binary table whose imaging_data sectionĬontains the masks described above. If there is more than one file they should be separatedīy spaces and included between double quotes: "file1 file2 file3" Were broken up into 100MB files by the on-line system. There may be more than one file because they "inFiles" a list of raw MIDI (PRISM/GRISM) input files representing ![]() Is a 1-dimensional spectrum for each window region. (perpendicular to the PRISM/GRISM dispersion). Not containing useful data) and summing in the y-direction Window by a floating point mask (which has zeros in rows oir1dCompressData "inFiles" maskFile outFileĬompress MIDI raw (PRISM/GRISM) files by multiplying each MIDI.More complete description of the C-language oirRoutines: Table-of-Contents C-routines IDL-Routines complexVisData = midiCVis(oirVisibilityStruct) keyValue = midiGetKeyword(keyword, inputFiles)ġ1. choppedData = midiChopImage(inputFiles)ġ0. sourceFlux = cdb->spectrumFromFile(fitsFile, diamData=diamData, specData=specData, rad=rad, /silent)ġ. sourceData = cdb->sourceFromFile(fitsFile, diamData=diamData, photData=photData, specData=specData, rad=rad, /silent)ħ. radii = cdb->sourcesNearPosition (ra, dec, sources, nmax=nmax, rmax=rmax)Ħ. nSource = cdb->sourceByAlias (alias, sourceData, diamData, photData, specData)ĥ. nSource = cdb->sourceByName (name, sourceData, diamData, photData, specData)Ĥ. Summary of calibration database routinesģ. simData=midiDecorrelate( targetdata, caldata, targtag, caltag, ratios.) midiProcess2Vis, targetFiles, calFiles, targTag, calTag, ,ġ0. Summary of IDL procedures that call the oirRoutines These are the "routine" routines that most people will use for standarized analysis of MIDI data.ġ. oirCrossCoeff baseName -cross outputFile -mask maskFile ġ7 oirCurveCal -A Afile -B Bfile -out outFile oirCalibrateVis targTag calTags ġ5 oirRescaleSpectra templateFile scaleFile outFileġ6. oirSci2HiPhot -AB ABfile -outbase outFileBase -ref refCoordFile -cross CrossCoeffFileġ4. oirMakePhotoSpectra -mask maskFile] -out outFile ġ2. oirChopPhotoImages -in "inFiles" -out outFile ġ1. oirAutoFlag infile delayFile flagFile ġ0. oirRotateGroupDelay infile delayFile outfile oir1dCompressData "inFiles" maskFile outFileĢ. Summary of C-language programs and calling sequences:ġ. ![]() Standard file names and contents used by scripts Description of file selection GUI (Gorgonzola) X. Summary of IDL Calibration Database Routines IV. Summary of IDL routines calling C routines(probably what you want to know!) III. That do most of the work and IDL front-ends for selecting Pronounced "Ooze") software for coherent estimation EWS - User Guide Previous: Processing Steps Up: Contents Next: File Formatsīelow a description of the EWS (Expert Work Station:
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