ACCOR | Corrects cross amplitudes using auto correlation measurements |
ACFIT | Determine antenna gains from autocorrelations |
ACLIP | edits suto-corr data for amplitudes, phases, and weights out of range |
ACSCL | Corrects cross amplitudes using auto correlation measurements |
ANCAL | Places antenna-based Tsys and gain corrections in CL table |
ANCHECK | Checks By sign in Antenna files |
ANTAB | Read amplitude calibration information into AIPS |
ANTENNAS | Antennas to include/exclude from the task or verb |
ANTUSE | Antennas to include/exclude from the task or verb |
ANTWT | Antenna Weights for UV data correction in Calibration |
APCAL | Apply TY and GC tables to generate an SN table |
APGPS | Apply GPS-derived ionospheric corrections |
ATMCA | Determines delay/phase gradient from calibrator observations |
BASELINE | specifies which antenna pairs are to be selected/deselected |
BASFIT | fits antenna locations from SN-table data |
BDAPL | Applies a BD table to another data set |
BLAPP | applies baseline-based fringe solutions a la BLAPP |
BLAVG | Average cross-polarized UV data over baselines. |
BLCAL | Compute closure offset corrections |
BLCHN | Compute closure offset corrections on a channel-by-channel basis |
BLING | find residual rate and delay on individual baselines |
BLPCL | Do divide by I,Q,U models for circular polarization BLCHN |
BLPLT | Plots BLCAL tables in 2 dimensions as function of baseline and IF |
BLPOLCAL | Do BLCHN for I, Q, U, V models |
BLVER | specifies the version of the baseline-calibration table used |
BPASS | computes spectral bandpass correction table |
BPASSPRM | Control adverb array for bandpass calibration |
BPCOR | Correct BP table. |
BPEDT | Interactive TV task to edit uv data based on BP tables |
BPEPL | Plots bandpass tables overlaying multiple times like BPEDT |
BPERR | Print and plot BPASS closure outputs |
BPFLG | Flgas uv data based on bad BP values |
BPLOT | Plots bandpass tables in 2 dimensions as function of time |
BPPLT | Plots selected contents of bandpass (BP) files versus time |
BPSMO | Smooths or interpolates bandpass tables to regular times |
BPVER | specifies the version of the bandpass table to be applied |
BPWAY | Determines channel-dependent relative weights |
BPWGT | Calibrates data and scales weights by bandpass correction |
BSPRT | print BS tables |
BSROT | modifies SD beam-switch continuum data for error in throw |
CALCODE | specifies the type of calibrator to be selected |
CALDIR | lists calibrator source models available as AIPS FITS files |
CALIB | determines antenna calibration: complex gain |
CALIBRAT | describes the process of data calibration in AIPS |
CALIN | specifies name of input disk file usually with calibration data |
CALMODEL | Applies SPLIT & UVSUB to make a model data set matching a calibrator |
CALRD | Reads calibrator source model-image FITS file |
CALSOUR | specifies source names to be included in calibration |
CC2IM | Make model image from a CC file |
CENTR | modifies UV data to center the reference channel |
CHANSEL | Array of start, stop, increment channel numbers to average |
CHREFANT | Name of reference antenna |
CLCAL | merges and smooths SN tables, applies them to CL tables |
CLCOP | copy CL/SN file calibration between polarizations or IFs |
CLCOR | applies user-selected corrections to the calibration CL table |
CLCORPRM | Parameter adverb array for task CLCOR |
CLINT | CL table entry interval |
CLINV | copy CL/SN file inverting the calibration |
CLIP | edits data based on amplitudes, phases, and weights out of range |
CLSMO | smooths a calibration CL table |
CLVLB | Corrects CL table gains for pointing offsets in VLBI data |
CMETHOD | specifies the method by which the uv model is computed |
CMODEL | specifies the method by which the uv model is computed |
CODETYPE | specifies the desired operation or data type |
CONFI | Optimize array configuration by minimum side lobes |
CPASS | computes polynomial spectral bandpass correction table |
CSCOR | applies specified corrections to CS tables |
CVEL | shifts spectral-line UV data to a given velocity |
DCHANSEL | Array of start, stop, increment channel #S + IF to avoid |
DECOR | Measures the decorrelation between channels and IF of uv data |
DEFLG | edits data based on decorrelation over channels and time |
DELCORR | Controls task actions on calibration tables. |
DELZN | Determines residual atmosphere depth at zenith and clock errors |
DFCOR | applies user-selected corrections to the calibration CL table |
DGAUS | Correct UV model for convolution by Clean beam |
DIGICOR | specifies whether VLBA digital corrections are to be applied |
DOACOR | specifies whether autocorrelation data are included |
DOAPPLY | Flag to indicate whether an operation is applied to the data |
DOBAND | specifies if/how bandpass calibration is applied |
DOBTWEEN | Controls smoothing between sources in calibration tables |
DOCALIB | specifies whether a gain table is to be applied or not |
DODELAY | selects solution for phase/amplitude or delay rate/phase |
DOFIT | Controls which antennas are fit by what methods |
DOFLAG | Controls closure cutoff in gain solutions and flagging |
DOOSRO | calibrating amplitude and phase, and imaging VLA data |
DOPOL | selects application of any polarization calibration |
DOVLAMP | Produces amp calibration file for phased-VLA VLBI data |
DT2PD | Write PD table from a PD table text file |
DTSIM | Generate fake UV data |
EDITA | Interactive TV task to edit uv data based on TY/SY/SN/CL tables |
EDITR | Interactive baseline-oriented visibility editor using the TV |
ELEVLIM | Lower limit on elevation |
ELFIT | Plots/fits selected contents of SN, TY, SY, PC or CL files |
ELINT | Determines and removes gain dependence on elevation |
EOPSFILE | Name of text file containing EOP information |
EVACL | Evaluates statistics in closure phase and amplitude |
EVASN | Evaluates statistics in SN/CL tables |
EVAUV | Subtracts & divides a model into UV data, does statistics on results |
FACES | makes images of catalog sources for initial calibration |
FARAD | add ionospheric Faraday rotation to CL table |
FGPLT | Plots selected contents of FG table |
FGPRT | Pprints counts of selected portions of an FG table |
FGTAB | writes frequency-range flags to a text file to be read by UVFLG |
FINDR | Find normal values for a uv data set |
FIXWT | Modify weights to reflect amplitude scatter of data |
FLAGR | Edit data based on internal RMS, amplitudes, weights |
FLAGVER | selects version of the flagging table to be applied |
FLGIT | flags data based on the rms of the spectrum |
FQTOL | Frequency tolerance with which FQ or frequency entries are accepted. |
FRCAL | Faraday rotation self calibration task |
FREQID | Frequency Identifier for frequency, bandwidth combination |
FRING | fringe fit data to determine antenna calibration, delay, rate |
FTFLG | interactive flagging of UV data in channel-time using the TV |
GAINERR | gives estimate of gain uncertainty for each antenna |
GAINUSE | specifies output gain table or gain table applied to data |
GAINVER | specifies the input gain table |
GCPLT | Plots gain curves from text files |
GCVER | specifies the version of the gain curve table used |
GETJY | determines calibrator flux densities |
GPSDL | Calculate ionospheric delay and Faraday rotation corrections |
HLPCLEAN | Cleaning tasks - run-time help |
HLPEDIBP | Interactive BP table uv-data editor BPEDT - run-time help |
HLPEDICL | Interactive SN/CL table uv-data editor - run-time help |
HLPEDIPC | Interactive PC table editor PCEDT - run-time help |
HLPEDIPD | Interactive PD table editor PDEDT - run-time help |
HLPEDISN | Interactive SN/CL table (not UV) editor - run-time help |
HLPEDISS | Interactive SY table (not UV) editor - run-time help |
HLPEDISY | Interactive SY table uv-data editor EDITA - run-time help |
HLPEDITS | Interactive TY table (not UV) editor - run-time help |
HLPEDITY | Interactive TY table uv-data editor EDITA - run-time help |
HLPEDIUV | Interactive uv-data editor EDITR - run-time help |
HLPFTFLG | Interactive time-channel visibility Editor - run-time help |
HLPIBLED | Interactive Baseline based visibility Editor - run-time help |
HLPPCFLG | Interactive time-channel PC table Editor PCFLG - 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 |
HLPSPFLG | Interactive time-channel visibility Editor SPFLG - run-time help |
HLPTVFLG | Interactive time-baseline visibility Editor TVFLG - run-time help |
HOLIS | Prints information about holography sampling |
IANTB | Writes out GC and TY data in ANTAB format |
IBLED | Interactive BaseLine based visibility EDitor |
ICHANSEL | Array of start, stop, increment channel #S + IF to average |
IM2CC | Task to convert an image to multi-facet Clean Components |
IMAGR | Wide-field and/or wide-frequency Cleaning / imaging task. |
IMFRING | large image delay fitting with IM2CC and OOFRING |
IMSCAL | large image self-cal with IM2CC and OOCAL |
INDXH | writes index file describing contents of UV data base |
INDXR | writes index file describing contents of UV data base |
INTERPOL | specifies the type of averaging done on the complex gains |
INTPARM | specifies the parameters of the frequency interpolation function |
KRING | fringe fit data to determine antenna calibration, delay, rate |
LDGPS | load GPS data from an ASCII file |
LISTR | prints contents of UV data sets and assoc. calibration tables |
LISUN | prints contents of UV data sets with Sun angles |
LOCIT | fits antenna locations from SN-table data |
LPCAL | Determines instrumental polarization for UV data |
MAPBM | Map VLA beam polarization |
MBDLY | Fits multiband delays from IF phases, updates SN table |
MFIMG | Image the Earth magnetic field model or TEC data used by TECOR |
MINAMPER | specifies the minimum amplitude error prior to some action |
MINANTEN | states minimum number of antennas for a solution |
MINPHSER | specifies the minimum phase error prior to some action |
MOD3D | Computes a 3D CC model from a set of facets |
MSORT | Sort a UV dataset into a specified order |
MULTI | Task to convert single-source to multi-source UV data |
NORMALIZ | specifies the type of gain normaliztion if any |
OMFIT | Fits sources and, optionally, a self-cal model to uv data |
ONEFREQ | states that the current CC model was made with one frequency |
OOCAL | determines antenna complex gain with frequency-dependent models |
OOFRING | Fringe fit data to determine calibration with spectral index options |
OOSRT | Sort a UV dataset into a specified order |
OOSUB | Subtracts/divides a model from/into a uv data base |
PBEAM | Fits the analytic function to the measured values of the beam |
PCABL | Copies the Cable cal values from PC table 1 to PC table n |
PCAL | Determines instrumental polarization for UV data |
PCASS | Finds amplitude bandpass shape from pulse-cal table data |
PCAVG | Averages pulse-cal (PC) tables over time |
PCCOR | Corrects phases using PCAL tones data from PC table |
PCDIV | Scales pulse-cal amplitudes by Tsys or Psum |
PCEDT | Interactive TV task to edit pulse-cal (PC) tables |
PCFIT | Finds delays and phases using a pulse-cal (PC) table |
PCFLG | interactive flagging of Pulse-cal data in channel-TB using the TV |
PCLOD | Reads ascii file containing pulse-cal info to PC table. |
PCPLT | Plots pulse-cal tables in 2 dimensions as function of time |
PCRMS | Finds statistics of a pulse-cal table; flags bad times and channels |
PCVEL | shifts spectral-line UV data to a given velocity: planet version |
PDEDT | Interactive TV task to edit polarization D-term (PD) tables |
PDPLT | Plots selected contents of PD tables |
PDVER | specifies the version of the spetral polarization table to use |
PEEK | fits pointing model function to output from the VLA |
PEELR | calibrates interfering sources in multi-facet imges |
PHASPRM | Phase data array, by antenna number. |
PIPEAIPS | calibrating amplitude and phase, and imaging VLA data |
POLANGLE | Intrinsic polarization angles for up to 30 sources |
POLSN | Make a SN table from cross polarized fringe fit |
PPAPP | Applies Right minus Left phase difference to a 2nd data set |
PRTSY | Task to print statistics from the SY table |
QUFIX | determines Right minus Left phase difference, corrects cal files |
QUOUT | writes text file of Q, U versus frequency to be used by RLDIF |
REAMP | Scale visibility amplitudes by IF- or subarray-dependent factor |
REFANT | Reference antenna |
RESEQ | Renumber antennas |
REWGT | modifies UV data re-scaling the weights only |
RFI | Look for RFI in uv data |
RLCAL | Determines instrumental right-left phase versus time (a self-cal) |
RLDIF | determines Right minus Left phase difference, corrects cal files |
RLDLY | fringe fit data to determine antenna R-L delay difference |
ROTMEAS | Tells the rotation measure of a source |
SAMPTYPE | Specifies sampling type |
SCIMG | Full-featured imaging plus self-calibration loop with editing |
SCMAP | Imaging plus self-calibration loop with editing |
SDCAL | Task to apply single dish calibration |
SDVEL | shifts spectral-line single-dish data to a given velocity |
SEARCH | Ordered list of antennas for fring searches |
SELBAND | SpecifieS bandwidth of the desired frequency ID |
SELFCAL | Requests self-calibration of calibration sources |
SELFREQ | SpecifieS frequency of desirde frequency ID |
SETJY | Task to enter source info into source (SU) table. |
SHAHO | Flags Holography data for shadowing |
SHOUV | displays uv data in various ways. |
SMODEL | Source model |
SMOTYPE | Specifies smoothing |
SMRATES | Requests smoothing and clipping of rates after FRING in pipeline |
SNBLP | Plots selected contents of SN or CL files on a baseline basis |
SNCOR | applies user-selected corrections to the calibration SN table |
SNCORPRM | Task-specific parameters for SNCOR. |
SNDUP | copies and duplicates SN table from single pol file to dual pol |
SNEDT | Interactive SN/CL/TY/SY table editor using the TV |
SNFIT | Fits parabola to SN amplitudes and plots result |
SNFLG | Writes flagging info based on the contents of SN files |
SNIFS | Plots selected contents of SN, TY, SY, PC or CL files by IF |
SNP2D | Task to convert SN table single-channel phase to delay |
SNPLT | Plots selected contents of SN, SY, TY, PC or CL files versus time |
SNREF | Chooses best reference antenna to minimize R-L differences |
SNRMS | Print statistics for selected contents of SN, SY, TY, PC or CL files |
SNSMO | smooths and filters a calibration SN table |
SNVER | specifies the output solution table |
SOLCL | adjust gains for solar data according to nominal sensitivity |
SOLCON | Gain solution constraint factor |
SOLINT | Solution interval |
SOLMIN | Minimum number of solution sub-intervals in a solution |
SOLMODE | Solution mode |
SOLSUB | Solution sub-interval |
SOLTYPE | Solution type |
SOUCODE | Calibrator code for source, not calibrator, selection |
SOUSP | fits source spectral index from SU table or adverbs |
SPCAL | Determines instrumental polzn. for spec. line UV data |
SPECINDX | Spectral index used to correct calibrations |
SPECPARM | Spectral index per polarization per source |
SPECTRAL | Flag to indicate whether an operation is spectral or continuum |
SPECURVE | Spectral index survature used to correct calibrations |
SPFLG | interactive flagging of UV data in channel-TB using the TV |
SPLAT | Applies calibration and splits or assemble selected sources. |
SPLIT | converts multi-source to single-source UV files w calibration |
SY2TY | Task to generate a TY extension file from an EVLA SY table |
SYPRT | Task to print values from the SY table |
SYSOL | undoes and re-does nominal sensitivity application for Solar data |
SYVSN | Plots selected SY/TY data with SN solution values versus time |
TASAV | Task to copy all extension tables to a dummy uv or map file |
TAU0 | Opacities by antenna number |
TDEPEND | Time-dependent imaging procedure sequence |
TECOR | Calculate ionospheric delay and Faraday rotation corrections |
TECRFILE | Name of file containg TEC data for use in TECOR |
TECRTYPE | Type of IONEX file to download in VLA and VLBA TECR procedures |
TEPLT | Plots selected contents of TE (TECOR) parameter tables |
TIMSMO | Specifiessmoothing times |
TLCAL | Converts JVLA telcal files to an SN file |
TRECVR | Receiver temperatures by polarization and antenna |
TRIANGLE | specifies closure triangles to be selected/deselected |
TRUEP | determines true antenna polarization from special data sets |
TVFLG | interactive flagging of UV data using the TV |
TYAPL | undoes and re-does nominal sensitivity application |
TYCOP | copy TY or SY table calibration between IFs |
TYSMO | smooths and filters a calibration TY or SY table |
TYSMOLEV | Clip level to use in running TYSMO on a VLB TY table |
TYVER | specifies the version of the system temperature table used |
UNCAL | sets up tables for uncalibrating Australia Telescope data |
USUBA | Assign subarrays within a uv-data file |
UVCRS | Finds the crossing points of UV-ellipses. |
UVFIT | Fits source models to uv data. |
UVFLG | Flags UV-data |
UVGIT | Fits source models to uv data. |
UVHOL | Prints holography data from a UV data base with calibration |
UVMLN | edits data based on the rms of the spectrum |
UVPRT | prints data from a UV data base with calibration |
UVSRT | Sort a UV dataset into a specified order |
UVSUB | Subtracts/divides a model from/into a uv data base |
VBCAL | Scale visibility amplitudes by antenna based constants |
VHCAL | Do divide by I,Q,U models for linear polarization data |
VHCALIB | Do CALIB for linear polarization with I, Q, U models |
VHDIF | find/apply V minus H linear polarization phase difference |
VHMOD | Compute linear polarization point source model, applies to data |
VLABP | VLA antenna beam polarization correction for snapshot images |
VLACALIB | Runs CALIB and LISTR for VLA observation |
VLACLCAL | Runs CLCAL and prints the results with LISTR |
VLALIST | Runs LISTR for VLA observation |
VLAMODE | VLA observing mode |
VLAMP | Makes ANTAB file for phased VLA used in VLBI observations |
VLANT | applies VLA/EVLA antenna position corrections from OPs files |
VLAOBS | Observing program or part of observer’s name |
VLAPROCS | Procedures to simplify the reduction of VLBA data |
VLARESET | Reset calibration tables to a virginal state |
VLARUN | Calibrating amplitude and phase, and imaging VLA data |
VLBAAMP | applies a-priori amplitude corrections to VLBA data |
VLBABPSS | computes spectral bandpass correction table |
VLBACALA | applies a-priori amplitude corrections to VLBA data |
VLBACCOR | applies a-priori amplitude corrections to VLBA data |
VLBACPOL | Procedure to calibrate cross-polarization delays |
VLBAEOPS | Corrects Earth orientation parameters |
VLBAFQS | Copies different FQIDS to separate files |
VLBAFRGP | Fringe fit phase referenced data and apply calibration |
VLBAFRNG | Fringe fit data and apply calibration |
VLBAKRGP | Fringe fit phase referenced data and apply calibration |
VLBAKRNG | Fringe fit data and apply calibration |
VLBAMCAL | Merges redundant calibration data |
VLBAMPCL | Calculates and applies manual instrumental phase calibration |
VLBAMPHC | applies VLBARUN calibration to additional phase stopping centers |
VLBAPANG | Corrects for parallactic angle |
VLBAPCOR | Calculates and applies instrumental phase calibration |
VLBARFI | Calibrates VLBA autocorrelations, writes out statistics |
VLBARUN | applies amplitude and phase calibration procs to VLBA data |
VLBATECR | Calculate ionospheric delay and Faraday rotation corrections |
VLBAUTIL | Procedures to simplify the reduction of VLBA data |
VLBAWIDE | Calibrates all VLA wide-band autocorrelations with VLBARFI |
VLBCD | Reads ascii file containing VLBA calibration info into a CD table |
VLBSY | Reads ascii file containing VLBA total power info into an SY table |
VLOG | Pre-process external VLBA calibration files |
WEIGHTIT | Controls modification of weights before gain/fringe solutions |
WETHR | Plots selected contents of WX tables, flags data based on WX |
WRTPROCS | Procedures to simplify the reduction of VLBA data |
WTTHRESH | defines the weight threshold for data acceptance |
WTUV | Specifies the weight to use for UV data outside UVRANGE |
WXLOD | Reads KEYIN-format weather information making WX table |
XYDIF | find/apply X minus Y linear polarization phase difference |
XYMOD | Compute linear polarization point source model, applies to data |