Date: Tue, 14 Jun 2011 17:21:11 -0400 (EDT)
From: Jun-Hui Zhao 
To: Jean Turner 
Subject: Re: installing miriad

Hi Jean,
    Great! You can play around the weighting to see if you can
optimize the imaging for the extended continuum emission.
    I have made a tarball for you.
http://www.cfa.harvard.edu/sma/miriad/data/jturner/

    This tarball contains a c-shell script (n5253.csh) for detailed
reduction of SMA data for N5253se CO(3-2) observations and the
calibrated datasets produced from executing this script:

110417_rx1.lsb.tsys.48.bp.ag.ch0 ->
         calibrated continuum uv for multiple sources from LSB
         (workable on CARMA Miriad)
110417_rx1.usb.tsys.48.bp.ag.ch0 ->
         calibrated continuum uv for multiple sources from USB
         (workable on CARMA Miriad)
n5253se.CO -> the uvdata set of the  CO(3-2) line + continuum
         in 48 spectral windows of 4GHz BW
         (may be not workable on CARMA Miriad becaused of 48windows)
n5253se.CO.uvlin -> the uvdata set of the  CO(3-2) line only
         (no continuum) in 48 spectral windows of 4GHz BW
         (may be not workable on CARMA Miriad becaused of 48windows)
n5253se.CO.vel -> the uvdata set that has converted to the
         velocity domain in velocity resolution 10 km/s
         (workable on CARMA Miriad)

You can use the script n5253.csh on CARMA Miriad for
1) continuum mapping: delete "#" in front of "goto CONTMAP"
   and excute this script,
2) line imaging: add "#" back to the front of "goto CONTMAP" and
   delete "#" in front of "goto LINMAP"; then
   and excute this script

This package also contains four example figures from this script.
    Jun-Hui





>Jun-Hui:  that is beautiful!!! that is what I was expecting, although I
>had expected more continuum away from the main source. wow.  --Jean