13.9 EDITING
\zxhlp{ACLIP} edits suto-corr data for amplitudes, phases, and weights out of range
\zxhlp{BPEDT} Interactive TV task to edit uv data based on BP tables
\zxhlp{BPFLG} Flgas uv data based on bad BP values
\zxhlp{CLIP} edits data based on amplitudes, phases, and weights out of range
\zxhlp{CROWDED} allows a task to perform its function in a crowded fashion
\zxhlp{DEFLG} edits data based on decorrelation over channels and time
\zxhlp{DOCLIP} Controls whether and how a \zxhlp{CLIP} operation is performed
\zxhlp{DOFLAG} Controls closure cutoff in gain solutions and flagging
\zxhlp{DOPLOT} Controls plotting of something
\zxhlp{DOROBUST} Controls method of averaging - simple mean/rms or robust
\zxhlp{EDITA} Interactive TV task to edit uv data based on TY/SY/SN/CL tables
\zxhlp{EDITR} Interactive baseline-oriented visibility editor using the TV
\zxhlp{EXPERT} specifies an user experience level or mode
\zxhlp{FGCNT} Counts samples comparing two flag tables
\zxhlp{FGDIF} Compares affect of 2 FG tables
\zxhlp{FGSPW} Flags bad spectral windows
\zxhlp{FGTAB} writes frequency-range flags to a text file to be read by \zxhlp{UVFLG}
\zxhlp{FINDR} Find normal values for a uv data set
\zxhlp{FLAGR} Edit data based on internal RMS, amplitudes, weights
\zxhlp{FLGIT} flags data based on the rms of the spectrum
\zxhlp{FTFLG} interactive flagging of UV data in channel-time using the TV
\zxhlp{GETITIME} Verb to return the UV data integration time.
HLPEDIBP Interactive BP table uv-data editor \zxhlp{BPEDT} - run-time help
HLPEDICL Interactive SN/CL table uv-data editor - run-time help
HLPEDIPC Interactive PC table editor \zxhlp{PCEDT} - run-time help
HLPEDIPD Interactive PD table editor \zxhlp{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 \zxhlp{EDITA} - run-time help
HLPEDITS Interactive TY table (not UV) editor - run-time help
HLPEDITY Interactive TY table uv-data editor \zxhlp{EDITA} - run-time help
HLPEDIUV Interactive uv-data editor \zxhlp{EDITR} - run-time help
HLPFTFLG Interactive time-channel visibility Editor - run-time help
HLPUFLAG Edit uv-data on a grid \zxhlp{UFLAG} - run-time help
HLPWIPER edit uv data from \zxhlp{UVPLT}-like plot \zxhlp{WIPER} - run-time help
\zxhlp{IBLED} Interactive BaseLine based visibility EDitor
\zxhlp{INTTIME} adds user-generated lines to the history extension file
\zxhlp{ISCALIB} states that the current source is a point-source calibrator
\zxhlp{NOISE} estimates the noise in images, noise level cutoff
\zxhlp{OFLAG} uses on-line flag table information to write a flag table
\zxhlp{OUTFGVER} selects version of the flagging table to be written
\zxhlp{PCEDT} Interactive TV task to edit pulse-cal (PC) tables
\zxhlp{PCFLG} interactive flagging of Pulse-cal data in channel-TB using the TV
\zxhlp{PDEDT} Interactive TV task to edit polarization D-term (PD) tables
\zxhlp{REASON} The reason for an operation
\zxhlp{REFLG} Attempts to compress a flag table
\zxhlp{RFI} Look for \zxhlp{RFI} in uv data
\zxhlp{RFLAG} Flags data set based on time and freq rms in fringe visibilities
\zxhlp{SCANLENG} specify length of "scan"
\zxhlp{SCIMG} Full-featured imaging plus self-calibration loop with editing
\zxhlp{SCMAP} Imaging plus self-calibration loop with editing
\zxhlp{SCUTOFF} noise level cutoff
\zxhlp{SDLSF} least squares fit to channels and subtracts from SD uv data
\zxhlp{SHAHO} Flags Holography data for shadowing
\zxhlp{SNEDT} Interactive SN/CL/TY/SY table editor using the TV
\zxhlp{SNFLG} Writes flagging info based on the contents of SN files
\zxhlp{SPFLG} interactive flagging of UV data in channel-TB using the TV
\zxhlp{TABED} Task to edit tables
\zxhlp{TAFLG} Flags data in a Table extension file
\zxhlp{TVFLG} interactive flagging of UV data using the TV
\zxhlp{UFLAG} Plots and edits data using a uv-plane grid and the TV
\zxhlp{UVFLG} Flags UV-data
\zxhlp{UVFND} prints selected data from UV data set to search for problems
\zxhlp{UVLIN} Fits and removes continuum visibility spectrum, also can flag
\zxhlp{UVLSD} least squares fit to channels and divides the uv data.
\zxhlp{UVLSF} least squares fit to channels and subtracts from uv data.
\zxhlp{UVMLN} edits data based on the rms of the spectrum
\zxhlp{VPFLG} Resets flagging to all or all corss-hand whenever some are flagged
\zxhlp{WETHR} Plots selected contents of WX tables, flags data based on WX
\zxhlp{WIPER} plots and edits data from a UV data base using the TV