AIPS HELP file for SNFLG in 31DEC18
As of Tue Jan 16 4:42:29 2018
SNFLG: writes flags based on discrepant solutions in SN files
INNAME UV data (name).
INCLASS UV data (class).
INSEQ 0.0 9999.0 UV data (seq. #). 0 => high
INDISK 0.0 9.0 Disk unit #. 0 => any
INEXT Input'SN' or 'CL' table
INVERS Input table file version no.
SOURCES Source list
QUAL -10.0 Source qualifier -1=>all
TIMERANG Time range to consider
STOKES Stokes type to consider
SELBAND Bandwidth to include (kHz)
SELFREQ Frequency to include (MHz)
FREQID Freq. ID to include, -1=>all
BIF 0.0 100.0 First IF to consider, 0=>1.
EIF 0.0 100.0 Last IF to consider
DOSTOKES -1.0 1.0 > 0 -> flag all Stokes if
one is bad
DOIFS -1.0 1.0 > 0 -> flag all IFs if one
SUBARRAY 0.0 Subarray to consider 0=>all
ANTENNAS Antennas to consider 0=>all
CUTOFF Table weight below which data
will not be considered, 0 =>
FLAGVER -1.0 FG table to be copied and
updated. -1 -> none.
OPTYPE What is examined: JUMP, AMP
DPARM Control parameters
(1) JUMP: max allowed phase
(1) AMP : max allowed
deviation from mean
(2) both: time interval (sec)
Usually a bit <- SOLINT
(1-6) A&P: min,max amp,
min,max phase, min,max wt
(7) A&P: > 0 -> flag all
antennas where one is bad
Use: Writes flagging info based on discrepencies in the SN table
solutions. OPTYPE='JUMP' flags on phase differences between
adjacent entries in SN files on a baseline-by-baseline basis.
It also writes flags to flag data before the first SN/CL table
record and after the last SN/CL record, but only if TIMERANGE
is not set. Furthermore, whenever a solution for a particular
antenna is marked bad or its weight is too low, a flag is
written to extend 70 percent of the way (in time) to the next good
solution (or all the way if both solutions are bad).
OPTYPE='AMP' finds the mean gain amplitude and rms separately
for each source, antenna, IF, and polarization. It then
produces flags for all solutions more than DPARM(1) * rms away
from the mean.
OPTYPE='A&P' examines every solution and generates flags for
those amplitudes < DPARM(1) or > DPARM(2), and phases <
DPARM(3) or > DPARM(4) in degrees (where phase runs from -180
to +180 degrees.
This task (OPTYPE='JUMP') was initially contributed by Lincoln
Greenhill and is based on a task initially designed by Mark
Reid, both of CfA.
INNAME.....UV file name (name). Standard defaults.
INCLASS....UV file name (class). Standard defaults.
INSEQ......UV file name (seq. #). 0 => highest.
INDISK.....Disk unit #. 0 => any.
INEXT......'SN' or 'CL' table to be consider
INVERS.....Version number of table to consider, 0=>highest no.
SOURCES....Source list. '*' = all; a "-" before a source name means
all except ANY source named. 'ALL' means to ignore the
source identifier in the SN/CL table and combine all of
them into one "source".
QUAL.......Only sources with a source qualifier number in the SU
table matching QUAL will be used if QUAL is not -1.
TIMERANG...Time range of the data to be considered. In order:
Start day, hour, min. sec, end day, hour, min. sec. Days
relative to reference date.
STOKES.....The desired Stokes type to be considered:
STOKES = 'V' or 'DIFF' gets you the phase difference of R
and L treated as the data for JUMP or the ratio of R and
L gains treated as the data for AMP. For A&P both
polarizations are considered with these STOKES values.
'R' = RCP only, 'L' = LCP only, else both.
SELBAND....Bandwidth of data to be selected. If more than one IF is
present SELBAND is the width of the first IF required.
Units = kHz.
SELFREQ....Frequency of data to be selected. If more than one IF is
present SELFREQ is the frequency of the first IF
required. Units = MHz.
FREQID.....Frequency identifier to select (you may determine which
is applicable from the OPTYPE='SCAN' listing produced by
LISTR). If either SELBAND or SELFREQ are set, their
values overide that of FREQID. However, setting SELBAND
and SELFREQ may result in an ambiguity. In that case,
the task will request that you use FREQID. -1 => all,
0 => first
BIF........Lowest IF to consider. 0 -> 1
EIF........Highest IF to consider. 0 -> highest
DOSTOKES...> 0 => flag all Stokes if one is bad
DOIFS......> 0 => flag all IFs if one is bad
SUBARRAY...Limit operation to specified subarray. 0 -> all
ANTENNAS...A list of the antennas to be considered. All 0 => all.
If any number is negative then all antennas listed are
NOT to be considered and all others are.
CUTOFF.....If >= 0, the task will examine the weight column of the
table and if the weight < CUTOFF, the task will consider
that sample to be bad. All samples with weight <= 0 are
considered bad. An FG table entry will be generated for
the time surrounding a bad solution.
CUTOFF is ignored for 'A&P' except as a default for
FLAGVER....Input FG version number. This FLAGVER will be copied to
a new version and the new flags appended to it. 0 ->
highest, -1 => none.
OPTYPE.....'JUMP' to flag based on jumps in the SN phases on a
baseline basis. 'AMP' to flag on gain amplitudes more
than DPARM(1) * rms away from the robust mean.
'A&P' to flag on solutions outside specified ranges in
amplitude, phase, and weight.
(1) Flag solution times > DPARM(1) * rms of that
antenna, source, IF, and polarization. 0 -> 6
Note that these mean and rms values are robust,
ignoring outliers. Deleting at 3 sigma is
(2) Time range around solution time to be flagged.
Usually the SOLINT as in JUMP. The time range is
the central time minus DPARM(2)/2 to the central
time plus DPARM(2)/2.
(1) Lowest allowed gain: 0 -> 0.
(2) Highest allowed gain: 0 -> 9999
(3) Lowest allowed phase: 0 -> -200
(4) Highest allowed phase: 0 -> +200
(5) Lowest allowed weight: 0 -> CUTOFF
(6) Highest allowed weight: 0 -> 999999
(7) > 0 => flag all antennas in the IF and
polarization when one antenna is bad.
'JUMP' or any other OPTYPE
(1) Maximum allowed phase jump between adjacent SN
(2) Minimum time interval over which to judge jumps
(sec). Times within DPARM(2) of each other are
regarded as the same. It is important that
DPARM(2) be less than any time difference between
two independent solutions in the SN table.
Notes from Lincoln Greenhill re JUMP:
The idea of flagging based on baseline-dependent jumps in phase does
seem counter to the AIPS philosophy. However, we think of it as
UV data is available in baseline-dependent terms. At time T0 and T1,
two contributing stations could have atmospheric solutions that jump
by reasonable amount, say +/-35 deg. However, this could correspond to
70 deg of jump on the corresponding baseline. The UV data between T0
and T1 must be calibrated in the context of this baseline-dependent
phase jump (since the SN entries are differenced). If that jump is
more than say 1 rad, then at times between T0 and T1, a linear
interpolation could be sufficiently discrepant from the true
atmospheric phase contribution as to contribute a fractional
Conversely, two stations could jump by +70 deg. This would be grounds
for flagging (if 1 rad is the threshold). But the difference is 0 and
there is no jump on the corresponding baseline. This data should be
OK. I could introduce a case in which the atmosphere is well
correlated over two antennas but otherwise highly variable. The
baseline-dependent phase jump from T0 to T1 would be 0 and the data
good. The antenna dependent phase jump from T0 to T1 would be