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Basic Information on uvpflag
Task: uvpflag
Purpose: Flag correlations of certain polarizations when template
Categories: calibration
UVPFLAG will flag all correlations of specified polarizations
when ALL given template polarizations are flagged. This can be
useful, for example, if you run TVFLAG, and flag data based upon
the XX correlation. You then use UVPFLAG and flag all other
correlations of the same baseline and time when the XX correlations
are flagged.
Key: vis
Input visibility file. No default.
Key: polt
Template polarizations. No default. Can be upto 4 polarizations
separated by commas from the following list:
xx, yy, xy, yx, rr, ll, rl, lr, i, q, u, v
Key: pols
Slave polarizations to flag when ALL template polarizations
are bad. No default. Choose up to 4 from the list given
for keyword `polt'.
Key: options
Task enrichment options. Minimum match is active.
or By default, UVPFLAG flags the slaves when ALL
of the templates are flagged. This option
directs it to flag the slaves when ANY one of
the templates are flagged.
full Instructs UVPFLAG to tell you about every record
it flags. The default is a summary at the end.
Generated by miriad@atnf.csiro.au on 21 Jun 2016