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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