Content-type: text/html Manpage of panda

panda

Section: User Commands (1)
Index Return to Main Contents
 

NAME

panda - Compute phase correction for each baseline, based on  

PERSON RESPONSIBLE

lmp  

CATEGORIES

uv analysis  

DESCRIPTION

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 interval.  

PARAMETERS

vis
CARMA visibility file to be calibrated. No default.
ref
SZA delay table (a .txt file for the moment). No default.
out
The name of the output uv data set. No default.
interval
Solution time interval, in minutes. The default is 0 minutes, i.e. no averaging.
list1
List of CARMA antennas to be paired with SZA. No default.
list2
List of SZA antennas, that are paired with 'list1'. No default.


 

Index

NAME
PERSON RESPONSIBLE
CATEGORIES
DESCRIPTION
PARAMETERS

This document was created by man2html, using the manual pages.
Time: 18:35:38 GMT, July 05, 2011