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13.19 MODELING

ACTNOISE    puts estimate of actual image uncertainty and zero in header
AGAUS    Fits 1-dimensional Gaussians to absorption-line spectra
BLPCL    Do divide by I,Q,U models for circular polarization BLCHN
BLPOLCAL    Do BLCHN for I, Q, U, V models
BOXES    Adds Clean boxes to BOXFILE around sources.
BSMOD    creates single-dish UV beam-switched data with model sources
BSTST    Graphical display of solutions to frequency-switched data
CHEBI    Make text file to plot Chebyshev polynomials
CMETHOD    specifies the method by which the uv model is computed
CMODEL    specifies the method by which the uv model is computed
CONFI    Optimize array configuration by minimum side lobes
CUBIT    Model a galaxy’s density and velocity distribution from full cube
DGAUS    Correct UV model for convolution by Clean beam
DIFUV    Difference two matching uv data sets, write out or print statistics
DOMODEL    selects display of model function
DORESID    selects display of differences between model and data
DOSPIX    selects solutions for spectral index of model components
EFACTOR    scales some error analysis process
EVAUV    Subtracts & divides a model into UV data, does statistics on results
FACES    makes images of catalog sources for initial calibration
FITOUT    specifies name of output text file for results of fitting
FSHIFT    specifies a position shift - output from fitting routines
FTARS    Fits 1-dimensional polarization spectrum to Q/U text file
GLENS    models galaxy gravitational lens acting on 3 component source
HLPAGAUS    Interactive Gaussian absorption fitting task AGAUS - run-time help
HLPLISPX    Fits spectral index model to data in text file - run-time help
HLPRMFIT    Polarization fitting task RMFIT - run-time help
HLPTVSAD    Find & fit Gaussians to an image with interaction - run-time help
HLPTVSPX    Fits 1-dimensional spectral index model to data - run-time help
HLPXGAUS    Interactive Gaussian fitting task XGAUS - run-time help
HLPZAMAN    Fits 1-dimensional Zeeman model to absorption data - run-time help
HLPZEMAN    Fits 1-dimensional Zeeman model to data - run-time help
IM2TX    Sums an image region into a 1-dimensional text file
IMFIT    Fits Gaussians to portions of an image
IMMOD    adds images of model objects to an image
INLIST    specifies name of input disk file, usually a source list
JMFIT    Fits Gaussians to portions of an image
MFITSET    gets adverbs for running IMFIT and JMFIT
MFPRT    prints MF tables in a format needed by modelling software
MOD3D    Computes a 3D CC model from a set of facets
MODAB    Makes simple absorption/emission spectral-line image in I/V
MODIM    adds images of model objects to image cubes in IQU polarization
MODSP    adds images of model objects to image cubes in I/V polarization
MODVF    task to create a warped velocity field
OMFIT    Fits sources and, optionally, a self-cal model to uv data
ONEFREQ    states that the current CC model was made with one frequency
OOSUB    Subtracts/divides a model from/into a uv data base
RADIUS    Specify a radius in an image
RM2PL    Plots spectrum of a pixel with RMFIT fit
RMFIT    Fits 1-dimensional polarization spectrum to Q/U cube
RMSLIMIT    selects things with RMS above this limit
SAD    Finds and fits Gaussians to portions of an image
SDMOD    modifies single-dish UV data with model sources
SLFIT    Task to fit gaussians to slice data.
SPMOD    Modify UV database by adding a model with spectral lines
SPXMD    adds images of model objects to image cubes in spectral index
STVERS    star display table version number
TK1SET    Verb to reset 1D gaussian fitting initial guess.
TKAMODEL    Verb to add slice model display directly on TEK
TKARESID    Verb to add slice model residuals directly on TEK
TKGUESS    Verb to display slice model guess directly on TEK
TKMODEL    Verb to display slice model directly on TEK
TKRESID    Verb to display slice model residuals directly on TEK
TKSET    Verb to set 1D gaussian fitting initial guesses.
TKSLICE    Verb to display slice file directly on TEK
TV1SET    Verb to reset 1D gaussian fitting initial guess on TV plot.
TVACOMPS    Verb to add slice model components directly on TV graphics
TVAGUESS    Verb to re-plot slice model guess directly on TV graphics
TVAMODEL    Verb to add slice model display directly on TV graphics
TVARESID    Verb to add slice model residuals directly on TV graphics
TVASLICE    Verb to add a slice display on TV graphics from slice file
TVCOMPS    Verb to display slice model components directly on TV graphics
TVGUESS    Verb to display slice model guess directly on TV graphics
TVMODEL    Verb to display slice model directly on TV graphics
TVRESID    Verb to display slice model residuals directly on TV graphics
TVSAD    Finds and fits Gaussians to portions of an image with interaction
TVSET    Verb to set slice Gaussian fitting initial guesses from TV plot
TVSLICE    Verb to display slice file directly on TV
TX2IM    Converts a 1-dimensional text file into cataloged image
UVFIT    Fits source models to uv data.
UVGIT    Fits source models to uv data.
UVMOD    Modify UV database by adding a model incl spectral index
UVSUB    Subtracts/divides a model from/into a uv data base
VHCAL    Do divide by I,Q,U models for linear polarization data
VHCALIB    Do CALIB for linear polarization with I, Q, U models
XG2PL    Plots spectrum of a pixel with XGAUS/AGAUS and ZEMAN/ZAMAN fits
XG2XG    Changes number of components in an XG or ZE table creating new one
XGAUS    Fits 1-dimensional Gaussians to images: restartable
ZAMAN    Fits 1-dimensional Zeeman model to absorption-line data
ZEMAN    Fits 1-dimensional Zeeman model to data

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