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 |
CUBIT | Model a galaxy’s density and velocity distribution from full cube |
DGAUS | Correct UV model for convolution by Clean beam |
DIFUV | Outputs the difference of two matching input uv data sets |
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 |
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 |
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 |
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