Manpage of panda
Section: User Commands (1)
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panda - Compute phase correction for each baseline, based on
This routine applies an atmospheric phase correction to a CARMA visibility dataset.
The phase correction is computed from the SZA delay table obtained from 'bldelay', and
applied in a baseline-based sense, with the possibility of averaging delays over a fixed
CARMA visibility file to be calibrated. No default.
SZA delay table (a .txt file for the moment). No default.
The name of the output uv data set. No default.
Solution time interval, in minutes. The default is 0 minutes, i.e. no averaging.
List of CARMA antennas to be paired with SZA. No default.
List of SZA antennas, that are paired with 'list1'. No default.
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Time: 18:35:38 GMT, July 05, 2011