Source
##########################################################################
# #
# Use Case Script for NGC 5921 #
# #
# Converted by STM 2007-05-26 #
# Updated STM 2007-06-15 (Alpha Patch 1) #
# Updated STM 2007-09-05 (Alpha Patch 2+) #
# Updated STM 2007-09-18 (Alpha Patch 2+) #
# Updated STM 2007-09-18 (Pre-Beta) add immoments #
# Updated STM 2007-10-04 (Beta) update #
# Updated STM 2007-10-10 (Beta) add export #
# Updated STM 2007-11-08 (Beta Patch 0.5) add RRusk stuff #
# Updated STM 2008-03-25 (Beta Patch 1.0) #
# Updated STM 2008-05-23 (Beta Patch 2.0) new tasking/clean/cal #
# Updated STM 2008-06-11 (Beta Patch 2.0) #
# #
# Features Tested: #
# The script illustrates end-to-end processing with CASA #
# as depicted in the following flow-chart. #
# #
# Filenames will have the <prefix> = 'ngc5921.usecase' #
# #
# Input Data Process Output Data #
# #
# NGC5921.fits --> importuvfits --> <prefix>.ms + #
# (1.4GHz, | <prefix>.ms.flagversions #
# 63 sp chan, v #
# D-array) listobs --> casa.log #
# | #
# v #
# flagautocorr #
# | #
# v #
# setjy #
# | #
# v #
# bandpass --> <prefix>.bcal #
# | #
# v #
# gaincal --> <prefix>.gcal #
# | #
# v #
# fluxscale --> <prefix>.fluxscale #
# | #
# v #
# applycal --> <prefix>.ms #
# | #
# v #
# split --> <prefix>.cal.split.ms #
# | #
# v #
# split --> <prefix>.src.split.ms #
# | #
# v #
# exportuvfits --> <prefix>.split.uvfits #
# | #
# v #
# uvcontsub --> <prefix>.ms.cont + #
# | <prefix>.ms.contsub #
# v #
# clean --> <prefix>.clean.image + #
# | <prefix>.clean.model + #
# | <prefix>.clean.residual #