source: trunk/InputComplete @ 1441

# FULL PARAMETER LIST
# -------------------
# 
# This file contains the full list of user-definable parameters. They are 
# grouped here according to their use, and the values quoted are the defaults:
# if a given parameter is not included in your parameter file, this is the 
# value it will take.
#
# In the comments at the start of each section, each parameter is listed followed 
# by its datatype (in []) and, where applicable, a description of the allowed range
# of values or types of inputs accepted (in {}), followed by a more verbose description.
#
#
### INPUT RELATED
#* imageFile [string] {filename (must exist)} -- The FITS image.  THERE IS NO DEFAULT FOR THIS.
#* flagSubsection [bool] {true or false, or 1 or 0} -- Whether to get a subsection of that image. 
#* subsection [string] {Subsection specification like [x1:x2,y1:y2,z1:z2]} -- The subsection to read in, in format [x1:x2,y1:y2,z1:z2], or * to indicate the full range 
#* flagReconExists [bool] {true or false, or 1 or 0} -- Set to true if the reconstructed cube exists as a FITS file (ie. it has been saved from a previous Duchamp run)
#* reconFile [string] {filename (must exist)} -- The location of the FITS file containing the reconstructed cube
#* flagSmoothExists [bool] {true or false, or 1 or 0} -- Set to true if the smoothed cube exists as a FITS file (ie. it has been saved from a previous Duchamp run)
#* smoothFile [string] {filename (must exist)} -- The location of the FITS file containing the smoothed cube
#* usePrevious [bool] {true or false, or 1 or 0} -- Whether to read the list of detected objects from a previously-created log file
#* objectList [string] {comma-separated list of object numbers (integers)} -- The list of objects to plot in individual plots: used with usePrevious=true

imageFile        your-file-here
flagSubsection   false
subsection       ""
flagReconExists  false
reconFile        your-reconstructed-file-here
flagSmoothExists false
smoothFile       your-smoothed-file-here
usePrevious      false
objectList       *

### OUTPUT RELATED
#* flagLog [bool] {true or false, or 1 or 0} -- Log the intermediate results?   
#* logfile [string] {filename} -- The file to put that in.
#* outFile [string] {filename} -- The final output list. 
#* flagSeparateHeader [bool] {true or false, or 1 or 0} -- Whether to write the header information (i.e. parameters, statistics and number of detections) to a separate file from the outFile (so that the outFile just contains the table of detections).
#* headerFile [string] {filename} -- The file to write the header information to.
#* flagWriteBinaryCatalogue [bool] {true or false, or 1 or 0} -- Whether to create a binary catalogue indicating the pixel locations of detected objects (for later reuse)
#* binaryCatalogue [string] {filename} -- The file containing the binary source catalogue
#* flagPlotSpectra [bool] {true or false, or 1 or 0} -- Whether to produce a file showing spectra of each detection
#* spectraFile [string] {filename} -- The postscript file of spectra
#* flagPlotIndividualSpectra [bool] {true or false, or 1 or 0} -- Whether to also write individual source spectra postscript files
#* flagTextSpectra [bool] {true or false, or 1 or 0} -- Whether to save a text file detailing the spectra of each source
#* spectraTextFile [string] {filename} -- The file in which to save the text-formatted spectra
#* flagOutputBaseline [bool] {true or false, or 1 or 0} -- Whether to save a FITS file containing the cube of baseline values
#* fileOutputBaseline [string] {filename} -- The filename for the baseline FITS file. If not given, it defaults to the format shown (for input file image.fits)
#* flagOutputMomentMap [bool] {true or false, or 1 or 0} -- Whether to save a FITS file containing the moment-0 map
#* fileOutputMomentMap [string] {filename} -- The filename for the moment-0 FITS file. If not given, it defaults to the format shown (for input file image.fits)
#* flagOutputMomentMask [bool] {true or false, or 1 or 0} -- Whether to save a FITS file containing the moment-0 mask image
#* fileOutputMomentMask [string] {filename} -- The filename for the moment-0 mask FITS file. If not given, it defaults to the format shown (for input file image.fits)
#* flagOutputMask [bool] {true or false, or 1 or 0} -- Whether to save a FITS file containing a mask array, showing the locations of detected objects
#* fileOutputMask [string] {filename} -- The filename for the mask file. If not given, it defaults to the format shown (for input file image.fits)
#* flagMaskWithObjectNum [bool] {true or false, or 1 or 0} -- If true, the detected pixels in the mask array have the object ID number, else they all have the value 1.
#* flagOutputSmooth [bool] {true or false, or 1 or 0} -- Whether to save the smoothed arrays as a FITS file
#* fileOutputSmooth [string] {filename} -- The filename for the smoothed array file. If not given, it defaults to the format shown (for input file image.fits). See documentation for explanation of format.
#* flagOutputRecon/Resid [bool] {true or false, or 1 or 0} -- Whether to save the reconstruction & residual arrays as FITS files
#* fileOutputRecon/Resid [string] {filename} -- The filename for the reconstruction or residual files. If not given, it defaults to the format shown (for input file image.fits). See documentation for explanation of format.
#* flagVOT [bool] {true or false, or 1 or 0} -- Make a VOTable file of the results?  
#* votFile [string] {filename} -- The file to put it in
#* flagKarma [bool] {true or false, or 1 or 0} -- Make a Karma annotation file of the results?  
#* karmaFile [string] {filename} -- The file to put it in
#* flagDS9 [bool] {true or false, or 1 or 0} -- Make a DS9 region file of the results?  
#* ds9File [string] {filename} -- The file to put it in
#* flagCasa [bool] {true or false, or 1 or 0} -- Make a CASA region file of the results?  
#* casaFile [string] {filename} -- The file to put it in
#* annotationType [string] {borders/circles/ellipses} -- Which type of annotation plot to use. Options are: borders = outline around detected pixels; circles = circle centred on object with radius encompassing all detected pixels; ellipses = ellipse centred on object with size given by MAJ, MIN, PA
#* flagMaps [bool] {true or false, or 1 or 0} -- Save postscript versions of the detection and 0th moment maps?
#* detectionMap [string] {filename}  -- The postscript file containing the detection map
#* momentMap [string] {filename} -- The postscript files containing the 0th-moment map
#* flagXOutput [bool] {true or false, or 1 or 0} -- Display the moment map in a pgplot window
#* newFluxUnits [string] {units, convertible from FITS file units} -- Brightness units to convert the array values to (eg. from Jy/beam to mJy/beam)   
#* precFlux [int] {>=0} -- Desired precision for Flux value in outputs.
#* precVel [int] {>=0} -- Desired precision for Velocity/Frequency value in outputs.
#* precSNR [int] {>=0} -- Desired precision for peak SNR value in ouputs.

flagLog                   false
logFile                   duchamp-Logfile.txt
outFile                   duchamp-Results.txt
flagSeparateHeader        false
headerFile                duchamp-Results.hdr
flagWriteBinaryCatalogue  true
binaryCatalogue           duchamp-Catalogue.dpc
flagPlotSpectra           true
spectraFile               duchamp-Spectra.ps
flagPlotIndividualSpectra false
flagTextSpectra           false
spectraTextFile           duchamp-Spectra.txt
flagOutputBaseline        false
fileOutputBaseline        image.BASE.fits
flagOutputMomentMap       false
fileOutputMomentMap       image.MOM0.fits
flagOutputMomentMask      false
fileOutputMomentMask      image.MOM0MASK.fits
flagOutputMask            false
fileOutputMask            image.MASK.fits
flagMaskWithObjectNum     false
flagOutputSmooth          false
fileOutputSmooth          image.SMOOTH-ND-X.fits
flagOutputRecon           false
fileOutputRecon           image.RECON-A-B-C-D.fits
flagOutputResid           false
fileOutputResid           image.RESID-A-B-C-D.fits
flagVOT                   false
votFile                   duchamp-Results.xml
flagKarma                 false
karmaFile                 duchamp-Results.ann
flagDS9                   false
ds9File                   duchamp-Results.reg
flagCasa                  false
casaFile                  duchamp-Results.crf
annotationType            borders
flagMaps                  true
detectionMap              duchamp-DetectionMap.ps
momentMap                 duchamp-MomentMap.ps
flagXOutput               true
newFluxUnits              no-default
precFlux                  3
precVel                   3
precSNR                   2

### MODIFYING THE CUBE
#* flagTrim [bool] {true or false, or 1 or 0} -- Whether to trim blank pixels from the edges of the cube.
#* flagBaseline [bool] {true or false, or 1 or 0} -- Whether to subtract spectral baselines before searching
#* flaggedChannels [string] {comma-separated list of channels} -- List of channels to ignore in the source-finding
#* baselineType [string] {either 'atrous' or 'median'} -- Which type of baseline estimation to use. Only 'atrous' or 'median' modes accepted.
#* baselineBoxWidth [int] {odd integer > 0} -- Box width used by the median baseline algorithm

flagTrim         false
flaggedChannels  ""
flagBaseline     false
baselineType     atrous
baselineBoxWidth 51

### GENERAL DETECTION RELATED
#* flagStatSec [bool] {true or false, or 1 or 0} -- Whether to only use a subsection of the cube to calculate the statistics.
#* StatSec [string] {Subsection specification like [x1:x2,y1:y2,z1:z2]} -- The subsection used for statistics calculations. It has the same format as the pixel subsection.
#* flagRobustStats [bool] {true or false, or 1 or 0} -- Shall we use robust statistics to characterise the noise in the image?
#* flagNegative [bool] {true or false, or 1 or 0} -- Are the features being searched for negative (set to true) or positive (false -- the default)?
#* snrCut [float] {any} --  How many sigma above mean is a detection when sigma-clipping
#* threshold [float] {any} -- The threshold flux dividing source and non-source. Used instead of calculating it from the cube's statistics. If not specified, it will be calculated.
#* flagGrowth [bool] {true or false, or 1 or 0} -- Should the detections be "grown" to a lower significance value?
#* growthCut [float] {any} -- The lower threshold used when growing detections
#* growthThreshold [float] {any} -- The lower threshold, used in conjunction with "threshold"
#* beamarea [float] {> 0.} -- The area of the beam in pixels (equivalent to the old beamsize parameter). This value is overridden by the BMAJ, BMIN, BPA header parameters if present.
#* beamFWHM [float] {> 0.} -- The full-width at half-maximum of the beam, in pixels. Where given, it overrides beamarea, but is overridden by the BMAJ, BMIN, BPA headers.
#* searchType [string] {either 'spatial' or 'spectral'} -- How the searching is done. Either "spatial", where each 2D map is searched then detections combined, or "spectral", where each 1D spectrum is searched then detections combined. 

flagStatSec     false
StatSec         ""
flagRobustStats true
flagNegative    false
snrCut          5.
threshold       0.
flagGrowth      false
growthCut       3.
growthThreshold 0.
beamArea        0.
beamFWHM        0.
searchType      spatial

### RECONSTRUCTION RELATED
#* flagATrous [bool] {true or false, or 1 or 0} -- Whether or not to do the reconstruction before searching
#* reconDim [int] {1, 2 or 3} -- The number of dimensions in which to perform the reconstruction.
#* scaleMin [int] {> 0} -- The minimum scale (starts at 1) to be included in the reconstruction
#* scaleMax [int] {any} -- The maximum scale to be included in the reconstruction. If it is <=0 then the maximum scale is calculated from the size of the array being reconstructed.
#* snrRecon [float] {> 0} -- The threshold used in filtering the wavelet coefficient arrays.
#* reconConvergence [float] {> 0.} -- The relative change in the residual rms must be less than this to stop the a trous iterations.
#* filterCode [int] {one of 1,2,3} -- The code number for the choice of filter to be used in the reconstruction:  1 = B3-spline filter, 2 = Triangle function, 3 = Haar wavelet. Other numbers default to 1.

flagATrous       false
reconDim         1
scaleMin         1
scaleMax         0
snrRecon         4.
reconConvergence 0.005
filterCode       1

### SMOOTHING
#* flagSmooth [bool] {true or false, or 1 or 0} -- Whether to smooth the cube.
#* smoothType [string] {either 'spectral' or 'spatial'} -- The type of smoothing to use, either "spectral" or "spatial"
#* hanningWidth [int] {> 0} -- The width parameter of the Hanning (spectral smoothing) function
#* kernMaj [float] {> 0.} -- The FWHM (in pixels) of the major axis of the 2D spatial smoothing gaussian
#* kernMin [float] {> 0.} -- The FWHM (in pixels) of the minor axis of the 2D spatial smoothing gaussian
#* kernPA [float] {any} -- The position angle (in degrees) of the major axis of the 2D spatial smoothing gaussian
#* smoothEdgeMethod [string] {one of 'equal', 'truncate' or 'scale'} -- How to deal with the pixels at the edge of the image when using the 2D smoothing algorith. Can be equal, truncate, or scale. 
#* spatialSmoothCutoff [float] {> 0.} -- Relative cutoff used to determine the width of the 2D smoothing kernel

flagSmooth           false
smoothType           spectral
hanningWidth         5
kernMaj              3.
kernMin              -1.
kernPA               0.
smoothEdgeMethod     equal
spatialSmoothCutoff  1.e-10

### FALSE DISCOVERY RATE METHOD
#* flagFDR [bool] {true or false, or 1 or 0} -- Whether or not to use the false discovery rate method instead of simple sigma clipping.
#* alphaFDR [float] {0. - 1.} -- The "alpha" parameter for the FDR method -- what desired fraction of discoveries will be false. Expressed as a decimal.
#* FDRnumCorChan [int] {>0} -- The number of neighbouring channels that are correlated. This is used only in the FDR algorithm

flagFDR         false
alphaFDR        0.01
FDRnumCorChan   2

### MERGING PARAMETERS
#* flagAdjacent [bool] {true or false, or 1 or 0} -- Whether to use the "adjacent criterion" to judge if objects are to be merged.
#* threshSpatial [float] {>= 0.} -- If flagAdjacent=false, this is the maximum spatial separation between objects for them to be merged.
#* threshVelocity [float] {>= 0.} -- The maximum channel separation between objects for them to be merged.
#* minChannels [int] {> 0} -- The minimum number of consecutive channels an object must have for it to be accepted.
#* minPix [int] {> 0} -- Minimum number of spatial pixels a detected object must have for it to be counted
#* minVoxels [int] {> 0} -- Minimum number of voxels a detected object must have for it to be counted
#* maxChannels [int] {any} -- The maximum number of channels an object must have for it to be accepted.
#* maxPix [int] {any} -- Maximum number of spatial pixels a detected object must have for it to be counted
#* maxVoxels [int] {any} -- Maximum number of voxels a detected object must have for it to be counted
#* flagRejectBeforeMerge [bool] {true or false, or 1 or 0} -- If true, reject sources for not meeting the above criteria before the merging stage
#* flagTwoStageMerging [bool] {true or false, or 1 or 0} -- If true, do an initial merge of a new source to the list (that is, merge it with the first source in the list that is close, but stop there)

flagAdjacent           true
threshSpatial          3
threshVelocity         7
minChannels            3
minPix                 2
minVoxels              4
maxChannels            -1
maxPix                 -1
maxVoxels              -1
flagRejectBeforeMerge  false
flagTwoStageMerging    true

### WCS PARAMETERS
#* spectralType [string] {a valid WCS type} -- An alternative spectral WCS type to use for spectral transformations.
#* restFrequency [float] {any} -- A value of the rest frequency to override any provided in the FITS header. Negative values will be ignored.
#* spectralUnits [string] {valid units string} -- What units you want the spectral axis to be plotted in and values quoted in (including the units of integrated flux)

spectralType   ""
restFrequency  -1
spectralUnits  ""

### OTHER PARAMETERS
#* verbose [bool] {true or false, or 1 or 0} -- Whether to provide progress indicators on the terminal during execution
#* drawBorders [bool] {true or false, or 1 or 0} -- Whether to draw borders around the detections on the moment maps in the output.
#* drawBlankEdges [bool] {true or false, or 1 or 0} -- Whether to draw an outline around any BLANK regions in the moment maps and image cutouts.
#* spectralMethod [string] {either 'peak' or 'sum'} -- How to plot the spectra in the output -- the spectrum of the peak pixel ("peak" -- the default), or integrated over all spatial pixels present ("sum")
#* pixelCentre [string] {one of 'centroid', 'average' or 'peak'} -- Which option to use for quoting the centre of the detection. Options are: centroid (flux-weighted average position), average (simple average with no weighting), peak (brightest pixel).
#* sortingParam [string] {one of 'xvalue', 'yvalue', 'zvalue', 'ra', 'dec', 'vel', 'w50', 'iflux',  'pflux', 'snr'} -- The parameter by which the final detection list is sorted

verbose         true
drawBorders     true
drawBlankEdges  true
spectralMethod  peak
pixelCentre     centroid
sortingParam    vel