AIPS HELP file for OUTFGVER in 31DEC22
As of Tue Sep 26 17:07:24 2023
Type: Adverb (Scalar)
Use: Selects the version of the flag table to be written.
In normal usage by editing tasks, FLAGVER selects the FG table
applied to the data on input. If OUTFGVER selects a new FG
table, then the flag commands from FLAGVER are copied to
OUTFGVER and then the new flags are appended. If OUTFGVER
selects an existing FG table (1 <= OUTFGVER <= FGmax), then the
new flags are appended to version OUTFGVER but the flags of
FLAGVER are not copied. If OUTFGVER <= 0 or OUTFGVER > FGmax,
then a new FG table will be written with version FGmax + 1.
A flag table may be applied to single-source or multi-source
data sets and may be applied to data which are not in time
order. If data are in time order, then flagging will work so
long as no more than 6000 flags apply to any one time. If the
data are not in time order, then flagging works only if no more
than 6000 flags apply to the current data. If you exceed these
limits, you may run UVCOP to apply the FG table so long as you
are within limits 10 times larger.
Null value: 0 => write a new flag table, but can vary with task.
ACLIP.....Edits suto-corr data for amplitudes, phases, and weights
out of range
BPEDT.....Interactive TV task to edit uv data based on BP tables.
BPFLG.....Flgas uv data based on bad BP values.
CLIP......Edits data based on amplitudes, phases, and weights out
CORER.....Calculates correlator statistics and flags bad ones.
DEFLG.....Edits data based on decorrelation over channels and time
EDITA.....Interactive TV task to edit uv data based on TY/SN/CL
EDITR.....Interactive baseline-oriented visibility editor using the
FGSPW.....Flags bad spectral windows.
FLAGR.....Edit data based on internal RMS, amplitudes, weights
FLGIT.....Flags data based on the rms of the spectrum
FTFLG.....Interactive flagging of UV data in channel-time using
IBLED.....Interactive BaseLine based visibility EDitor
OFLAG.....Uses on-line flag table information to write a flag table
REWAY.....Computes weights based in rms in spectra. Output flag
table is optional and is used when solutions are "bad".
RFLAG.....Flags data set based on time and freq rms in fringe
SCIMG.....Full-featured imaging plus self-calibration loop
SCMAP.....Imaging plus self-calibration loop
SHAHO.........Flags Holography data for shadowing
SPFLG.....Interactive flagging of UV data in channel-T using the TV
TVFLG.....Interactive flagging of UV data in TB using the TV
UFLAG.....Plots and edits data using a uv-plane grid and the TV.
UVMLN.....Edits data based on the rms of the spectrum
WETHR.....Plots selected contents of WX tables, flags data based on
WX (weather data)
WIPER.....Plots and edits data from a UV data base using the TV