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- BLANK : Blanks out non-signal portions of images.
- BLSUM : Sums images over blotch regions including spectra.
- CCMOD : Add model to CC list
- CLIP : Flag data whose amplitude is out of range.
- CNTR : Generate a contour plot as TV image or plot file.
- COMB : Combine in many ways two overlapping images.
- CONVL : Convolve an image.
- CVEL : Shift spectral line data to a given velocity
- FARAD : Add ionospheric Faraday rotation to CL table.
- GAL : Determine parameters from a velocity field.
- HGEOM : Make an image consistent with another image.
- IM2UV : FFT an image and convert to a UV data file.
- IMEAN : Print the mean, rms and extrema in an image.
- IMFIT : Fit gaussian models to an image.
- IMFLT : Flattens an image by fitting a plane to the image.
- IRING : Integrate in confocal ellipses.
- JMFIT : Fit Gaussian models to an image by least-squares.
- MAPIT : CLEAN and Self-Calibrate UVDATA.
- MATHS : Operate on an image with mathematical functions.
- MCUBE : Collect a set of n-dim maps into a (n+1)-dim map.
- MOMFT : Calculate moments of a component.
- MOMNT : Calculate profile moments.
- MWFLT : Applies a nonlinear lowpass filter to an image.
- NINER : Applies various 3x3 area operaters to an image.
- NNLSQ : Non-Negative-Least-Squares decomposition of spectrum
- PADIM : Increase image size by padding with some value
- PBCOR : Apply the primary beam correction.
- PCNTR : Generate plot file for contour plus pol. vectors
- PGEOM : Transform an image into polar coordinates.
- POLCO : Correct polarization maps for Ricean bias
- REGRD : Transforms image coordinate system and geometry.
- RM : Calculate rotation measure and magnetic field.
- SLFIT : Fit gaussians to slice data.
- SLICE : Make a slice file from an image.
- SMOTH : Smooth a subimage from upto a 7-dim. image.
- SQASH : Sums together or average planes in a cube.
- STESS : Finds sensitivity in mosaicing.
- STFUN : Calculate a structure function image.
- SUBIM : Select a subimage from upto a 7-dim. image.
- SUMIM : Sum overlapping, sequentially-numbered images.
- SUMSQ : Sum the squared pixel values of overlapping sequentially numbered images.
- UVFIT : Fit gaussian or spheres to UV data.
- UVLIN : Fit baselines to visibility spectra and subtract.
- UVLSF : Fit baselines to visibility spectra and subtract.
- UVMOD : Inserts a model into uv data.
- UVMTH : Corrects one uv dataset with the average of another.
- UVSEN : Determine rms sidelobe and sensitivity.
- UVSRT : Sorts UV data.
- UVSUB : Subtract CLEAN components from a uv data base.
- WARP : Model warps in galaxies.
- XBASL : Fits n'th order polynomials to rows of images.
- XGAUS : Fits 1-dimensional Gaussians to images.
- XMOM : Finds the moments of each row of an image.
- XSMTH : Smooth data on the x axis only.
- XSUM : Sum or average data on the x axis only.
- XTRAN : Create a new image with transformed coodinates
Next: Utility Tasks
Up: AVAILABLE TASKS in AIPS
Previous: Display Tasks
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