Documentation on uvdiff
Task: uvdiff
Purpose: Difference two visibility datasets.
Categories: uv analysis
Given two Miriad visibility datasets, UVDIFF matches and optionally
subtracts one from the other. In doing this, UVDIFF assumes that the
two datasets sample the same source using the same array configuration
and observing frequency setup (no checks are made to verify these).
UVDIFF matches visibility records based on baseline number,
polarisation type and hour angle. If the hour angles in the two
datasets do not match to better than 1 second, UVDIFF linearly
interpolates between two integrations of one dataset to the
appropriate hour angle of the other.
NOTE: UVDIFF does not apply calibration corrections to either
of the input datasets. The datasets should be in time order.
Key: vis
The two datasets to difference. No default. When differencing, the
output is the first minus the second. The first visibility dataset
is used as the template for the output. It is the second dataset
that is interpolated when needed.
Key: select
Standard visibility selection keyword. See the help on select for
more information. Note that this selection is applied ONLY to the
first visibility dataset. The default is to select everything.
Key: out
The output dataset. No default.
Key: mode
This determines what data is written. Possible values are:
difference Write the difference of the two inputs (the first
minus the second). This is the default.
two Write the data from the second input, interpolated
to the first.
one Write the first dataset.
With the exception of the visibility data itself, all three
possibilities will produce identical datasets. This includes
identical flagging information.
Key: tol
Interpolation tolerance, in minutes. This gives the maximum
gap between two integrations to interpolate across. The default is
2 minutes.
Generated by rsault@atnf.csiro.au on 11 Jul 1996