Documentation on gpboot
Task: gpboot
Purpose: Correct the gains table of a visibility data-set.
Categories: calibration
GpBoot is a MIRIAD program which corrects a visibility data-set's
gain table.
GpBoot works by comparing the amplitudes in the gain table of one
data-set with those of another. The gains are assumed to differ
by a constant factor. It is assumed that the
instrumental gain and atmospheric attenuation of the two data-sets
were the same, and so the difference in gain is due to an
arbitrary or incorrect flux being specified when initially
determining the gains.
GpBoot will also correct for differences in the XY phase offsets
between the two data-sets, and copy across the polarization
leakage parameters.
Key: vis
The input visibility file, containing the gain file to correct.
The gains and XY phases are assumed to be out by a constant
factor.
Key: cal
This is a visibility data-set, which is assumed to contain a
gain table which scales the data to absolute flux units, and
contains correct XY phases.
Key: select
Normal uv-selection parameter. This selects the gains in the
``vis'' that are compared against the ``cal'' gains (note that
all the ``cal'' gains are involved in the comparison). Currently
ONLY time selection is permitted. You will use this parameter
to select which time(s) the instrumental/atmospheric amplitude
gains for ``vis'' are comparable to the observation in ``cal''.
Key: options
This gives task enrichment parameters. Several can be given,
separated by commas. Minimum match is used.
"noxy" Do not correct for XY phase differences. The
default is to correct for this if the ``gains''
item is present in both data-sets.
"nocal" Do not correct the flux scale. The default is to
correct the flux scale if the ``gains'' item is
present in both data-sets.
Generated by rsault@atnf.csiro.au on 11 Jul 1996