AHIST | Task to convert image intensities by adaptive histogram |
ALLOKAY | specifies that initial conditions have been met. |
APCLN | Deconvolves images with CLEAN algorithm |
APGS | deconvolves image with Gerchberg-Saxton algorithm |
APVC | Deconvolves images with van Cittert algorithm |
AVOPTION | Controls type or range of averaging done by a task |
BCOMP | gives beginning component number for multiple fields |
BLC | gives lower-left-corner of selected subimage |
BLWUP | Blow up an image by any positive integer factor. |
BMAJ | gives major axis size of beam or component |
BMIN | gives minor axis size of beam or component |
BOX | specifies pixel coordinates of subarrays of an image |
BOX2CC | Converts CLBOX in pixels to CCBOX in arc seconds |
BOXES | Adds Clean boxes to BOXFILE around sources. |
BOXFILE | specifies name of Clean box text file |
BPA | gives position angle of major axis of beam or component |
BSAVG | Task to do an FFT-weighted sum of beam-switched images |
BSCLN | Hogbom Clean on beam-switched difference image |
BSGRD | Task to image beam-switched single-dish data |
BSMAP | images weak sources with closure phases |
CANDY | user-definable (paraform) task to create an AIPS image |
CCBOX | specifies pixel coordinates of subarrays of an image |
CCEDT | Select CC components in BOXes and above mininum flux. |
CCFND | prints the contents of a Clean Components extension file. |
CCGAU | Converts point CLEAN components to Gaussians |
CCMOD | generates clean components to fit specified source model |
CCMRG | sums all clean components at the same pixel |
CCRES | Removes or restores a CC file to a map with a gaussian beam. |
CELLSIZE | gives the pixel size in physical coordinates |
CHKFC | makes images of Clean boxes from Boxfile |
CLBOX | specifies subarrays of an image for Clean to search |
CMETHOD | specifies the method by which the uv model is computed |
CMODEL | specifies the method by which the uv model is computed |
COHER | Baseline Phase coherence measurement |
CONPL | Plots AIPS gridding convolution functions |
CONVL | convolves an image with a gaussian or another image |
CUTOFF | specifies a limit below or above which the operation ends |
CXCLN | Complex Hogbom CLEAN |
CXIMAGR | Grid UV data into a complex image, Fourier transform, Clean |
DCONV | deconvolves a gaussian from an image |
DECSHIFT | gives Y-coordinate shift of an image center from reference |
DELBOX | Verb to delete boxes with TV cursor & graphics display. |
DFILEBOX | Verb to delete Clean boxes with TV cursor & write to file |
DO3DIMAG | specifies whether uvw’s are reprojected to each field center |
DOGRIDCR | selects correction for gridding convolution function |
DOOSRO | calibrating amplitude and phase, and imaging VLA data |
DRAWBOX | Verb to draw Clean boxes on the display |
DTSUM | Task to provide a summary of the contents of a dataset |
EVAUV | Subtracts & divides a model into UV data, does statistics on results |
FACES | makes images of catalog sources for initial calibration |
FACTOR | scales some display or CLEANing process |
FETCH | Reads an image from an external text file. |
FFT | Takes Fourier Transform of an image or images |
FGAUSS | Minimum flux to Clean to by widths of Gaussian models |
FILEBOX | Verb to reset Clean boxes with TV cursor & write to file |
FILIT | Interactive BOXFILE editing with facet images |
FIXBX | converts a BOXFILE to another for input to IMAGR |
FLATN | Re-grid multiple fields into one image incl sensitivity |
FLDSIZE | specifies size(s) of images to be processed |
FLUX | gives a total intensity value for image/component or to limit |
FOV | Specifies the field of view |
FSHIFT | specifies a position shift - output from fitting routines |
FSIZE | file size in Megabytes |
GAIN | specifies loop gain for deconvolutions |
GUARD | portion of UV plane to receive no data in gridding |
HA2TI | Converts data processed by TI2HA (STUFFER) back to real times |
HISEQ | task to translate image by histogram equalization |
HLPCLEAN | Cleaning tasks - run-time help |
HLPSCIMG | Full-featured image plus self-cal loops, editing - run-time help |
HLPSCMAP | Imaging plus self-cal and editing SCMAP - run-time help |
HOCLN | Task to do a clean of holography images |
HOLGR | Read & process holography visibility data to telescope images |
HOLOG | Read & process holography visibility data to telescope images |
IM2CC | Task to convert an image to multi-facet Clean Components |
IM2PARM | Specifes enhancement parameters for OOP-based imaging: 2nd set |
IM2UV | converts an image to a visibility data set |
IMAGR | Wide-field and/or wide-frequency Cleaning / imaging task. |
IMAGRPRM | Specifes enhancement parameters for OOP-based imaging |
IMERG | merges images of different spatial resolutions |
IMSIZE | specifies number of pixels on X and Y axis of an image |
IMTXT | Write an image to an external text file. |
INLIST | specifies name of input disk file, usually a source list |
LINIMAGE | Build image cube from multi-IF data set |
LTESS | makes mosaic images by linear combination |
MANDL | creates an image of a subset of the Mandlebrot Set |
MAPPR | Simplified access to IMAGR |
MASKS | Makes mask image of Clean boxes from boxfile |
MAXPIXEL | maximum pixels searched for components in Clark CLEAN |
MOD3D | Computes a 3D CC model from a set of facets |
MODVF | task to create a warped velocity field |
MWFLT | applies linear & non-linear filters to images |
NBOXES | Number of boxes |
NCCBOX | Number of clean component boxes |
NCOMP | Number of CLEAN components |
NDIG | Number of digits to display |
NFIELD | The number of fields imaged |
NMAPS | Number of maps (images) in an operation |
NOIFS | makes all IFs into single spectrum |
NOISE | estimates the noise in images, noise level cutoff |
OBITIMAG | Access to OBIT task Imager without self-cal or peeling |
OBITMAP | Simplified access to OBIT task Imager |
OBITPEEL | Access to OBIT task Imager with self-cal and peeling |
OBITSCAL | Access to OBIT task Imager with self-cal, NOT peeling |
OBITVERS | Python version to use with BDF2AIPS and OBIT imaging verbs |
OBOXFILE | specifies name of output Clean box text file |
ONEBEAM | specifies whether one beam is made for all facets or one for each |
ONEFREQ | states that the current CC model was made with one frequency |
OOSUB | Subtracts/divides a model from/into a uv data base |
OUT2CLAS | The class of a secondary output file |
OUT2DISK | The disk number of a secondary output file. |
OUT2NAME | The name of a secondary output file. |
OUT2SEQ | The sequence of a secondary output file. |
OVERLAP | specifies how overlaps are to be handled |
OVRSWTCH | specifies when IMAGR switches from OVERLAP ¿= 2 to OVERLAP = 1 mode |
PADIM | Task to increase image size by padding with some value |
PASTE | Pastes a selected subimage of one image into another. |
PATGN | Task to create a user specified test or primary-beam pattern |
PBCOR | Task to apply or correct an image for a primary beam |
PBPARM | Primary beam parameters |
PBSIZE | estimates the primary beam size in interferometer images |
PGEOM | Task to transform an image into polar coordinates. |
PHASE | Baseline Phase coherence measurement |
PHAT | Prussian hat size |
PIPEAIPS | calibrating amplitude and phase, and imaging VLA data |
PIX2VAL | An image value in the units specified in the header. |
PIX2XY | Specifies a pixel in an image |
PIXAVG | Average image value |
PIXRANGE | Range of pixel values to display |
PIXSTD | RMS pixel deviation |
PIXVAL | Value of a pixel |
PIXXY | Specifies a pixel location. |
PRTCC | prints the contents of a Clean Components extension file. |
PUTVALUE | Verb to store a pixel value at specified position |
QCREATE | adverb controlling the way large files are created |
QUANTIZE | Quantization level to use |
REBOX | Verb to reset boxes with TV cursor & graphics display. |
REGRD | Regrids an image from one co-ordinate frame to another |
REMAG | Task to replace magic blanks with a user specified value |
RMSD | Calculate rms for each pixel using data in a box around the pixel |
ROBUST | Uniform weighting ”robustness” parameter |
RSTOR | Restores a Clean component file to a map with a Gaussian beam. |
SABOX | create box file from source islands in facet images |
SCIMG | Full-featured imaging plus self-calibration loop with editing |
SCMAP | Imaging plus self-calibration loop with editing |
SDCLN | deconvolves image by Clark and then ”SDI” cleaning methods |
SDGRD | Task to select and image random-position single-dish data |
SDIMG | Task to select and image random-position single-dish data |
SETFC | makes a BOXFILE for input to IMAGR |
SHADW | Generates the ”shadowed” representation of an image |
SHIFT | specifies a position shift |
SIZEFILE | return file size plus estimate of IMAGR work file size |
SKEW | Specifies a skew angle |
SKYVE | Regrids a DSS image from one co-ordinate frame to another |
SMODEL | Source model |
SNCUT | Specifies minimum signal-to-noise ratio |
SPCOR | Task to correct an image for a primary beam and spectral index |
SPECR | Spectral regridding task for UV data |
SPFIX | Makes cube from input to and output from SPIXR spectral index |
SPIXR | Fits spectral indexes to each row of an image incl curvature |
STACK | Task to co-add a set of 2-dimensional images with weighting |
STEER | Task which deconvolves the David Steer way. |
STESS | Task which finds sensitivity in mosaicing |
STFACTOR | scales star display or SDI CLEANing process |
STUFFR | averages together data sets in hour angle |
SUBIM | Task to select a subimage from up to a 7-dim. image |
SUMIM | Task to sum overlapping, sequentially-numbered images |
TDEPEND | Time-dependent imaging procedure sequence |
TDSCANS | Time-dependent imaging procedure sequence: find intervals |
TDSSCAN | Time-dependent imaging procedure sequence: find intervals |
TDSTEP3 | Time-dependent imaging procedure ”step 3” |
TDSTEP5 | Time-dependent imaging procedure sequence: later steps |
TKBOX | Procedure to set a Clean box with the TK cursor |
TKNBOXS | Procedure to set Clean boxes 1 - n with the TK cursor |
TRANS | Task to transpose a subimage of an up to 7-dim. image |
TRANSCOD | Specified desired transposition of an image |
TRC | Specified the top right corner of a subimage |
TVBOX | Verb to set boxes with TV cursor & graphics display. |
UBAVG | Baseline dependent time averaging of uv data |
UNSPX | Removes spectral index model from a data cube |
UTESS | deconvolves images by maximizing emptiness |
UVBOX | radius of the smoothing box used for uniform weighting |
UVBXFN | type of function used when counting for uniform weighting |
UVFRE | Makes one data set have the spectral structure of another |
UVIMG | Grid UV data into an ”image” |
UVMAP | makes images from calibrated UV data. |
UVPOL | modifies UV data to make complex image and beam |
UVSIZE | specifies number of pixels on X and Y axes of a UV image |
UVSUB | Subtracts/divides a model from/into a uv data base |
UVWTFN | Specify weighting function, Uniform or Natural |
VLARUN | Calibrating amplitude and phase, and imaging VLA data |
VTESS | Deconvolves sets of images by the Maximum Entropy Method |
WGAUSS | Widths of Gaussian models (FWHM) |
WTSUM | Task to do a a sum of images weighted by other images |
XMOM | Fits one-dimensional moments to each row of an image |
YPARM | Specifies Y axis convolving function |
ZEROSP | Specify how to include zero spacing fluxes in FT of UV data |