NGC3256Band3 for CASA 3.3: Difference between revisions

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==Overview==
==Overview==
[[File:OpticalImageNGC3256.jpg|200px|thumb|right|HST image of NGC3256 (credit: NASA, ESA, the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University))]]
[[File:OpticalImageNGC3256.jpg|200px|thumb|right|HST image of NGC3256 (credit: NASA, ESA, the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University))]]


NGC3256 is the most amazing galaxy ever [...blah blah blah, To be written by Eric]
[To be written by Eric]


==How to use this Casa Guide==
==How to use this Casa Guide==
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To start the data reduction process from the raw data, begin with the Calibration section: [[NGC3256 Band3 - Calibration]].  Once you have completed that section, or if you would like to skip over the calibration process, proceed to [[NGC3256 Band3 - Imaging]].
To start the data reduction process from the raw data, begin with the Calibration section: [[NGC3256 Band3 - Calibration]].  Once you have completed that section, or if you would like to skip over the calibration process, proceed to [[NGC3256 Band3 - Imaging]].


==Retrieving the Data==
For both portions of the guide, we will provide you with the full CASA commands needed to carry out each step.  Simply copy and paste the commands into your CASA terminal.  For more help getting started with CASA, see [that link about getting started in CASA…].
 
==Obtaining the Data==


====Raw Data====
The data were taken in six different datasets over two consecutive nights: April 16-17, 2011.  There are three datasets for April 16th and three for April 17th.  Here we provide you with "starter" datasets, where we have taken the raw data in ALMA Science Data Model (ASDM) format and converted them to CASA Measurement Sets (MS).  We did this using the {{importasdm}} task in CASA.   
The data were taken in six different datasets over two consecutive nights: April 16-17, 2011.  There are three datasets for April 16th and three for April 17th.  Here we provide you with "starter" datasets, where we have taken the raw data in ALMA Science Data Model (ASDM) format and converted them to CASA Measurement Sets (MS).  We did this using the {{importasdm}} task in CASA.   


[What else are we going to do to the data we provide?]
Along with the Measurement Sets, we also provide some tables that you will need for the calibration.  These include the System Temperature (Tsys) tables, which contain corrections for atmospheric opacity, and Water Vapor Radiometer (WVR) tables, which contain the atmospheric phase corrections determined by the water vapor radiometers on each antenna. 


Along with the Measurement Sets, we also provide some tables that you will need for the calibration.  These include the System Temperature (Tsys) tables, which contain corrections for atmospheric opacity, and Water Vapor Radiometer (WVR) tables, which contain the atmospheric phase corrections determined by the water vapor radiometers on each antenna.  
You can download the data here:
 
[LINK]
 
Once the download has finished, unpack the file:
<source lang="python">
# In a terminal outside CASA
tar -xvf ngc3256band3raw.tgz
</source>
 
====Calibrated Data====
 
For those wishing to skip the calibration section, we also provide the fully-calibrated data [on the science target, or everything?]  


You can download the data here:
You can download the data here:
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<source lang="python">
<source lang="python">
# In a terminal outside CASA
# In a terminal outside CASA
tar -xvf ngc3256band3.tgz
tar -xvf ngc3256band3cal.tgz
</source>
</source>

Revision as of 23:27, 23 May 2011

Overview

HST image of NGC3256 (credit: NASA, ESA, the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University))

[To be written by Eric]

How to use this Casa Guide

This CASA Guide consists of two parts:

NGC3256 Band3 - Calibration

NGC3256 Band3 - Imaging

To start the data reduction process from the raw data, begin with the Calibration section: NGC3256 Band3 - Calibration. Once you have completed that section, or if you would like to skip over the calibration process, proceed to NGC3256 Band3 - Imaging.

For both portions of the guide, we will provide you with the full CASA commands needed to carry out each step. Simply copy and paste the commands into your CASA terminal. For more help getting started with CASA, see [that link about getting started in CASA…].

Obtaining the Data

Raw Data

The data were taken in six different datasets over two consecutive nights: April 16-17, 2011. There are three datasets for April 16th and three for April 17th. Here we provide you with "starter" datasets, where we have taken the raw data in ALMA Science Data Model (ASDM) format and converted them to CASA Measurement Sets (MS). We did this using the importasdm task in CASA.

Along with the Measurement Sets, we also provide some tables that you will need for the calibration. These include the System Temperature (Tsys) tables, which contain corrections for atmospheric opacity, and Water Vapor Radiometer (WVR) tables, which contain the atmospheric phase corrections determined by the water vapor radiometers on each antenna.

You can download the data here:

[LINK]

Once the download has finished, unpack the file:

# In a terminal outside CASA
tar -xvf ngc3256band3raw.tgz

Calibrated Data

For those wishing to skip the calibration section, we also provide the fully-calibrated data [on the science target, or everything?]

You can download the data here:

[LINK]

Once the download has finished, unpack the file:

# In a terminal outside CASA
tar -xvf ngc3256band3cal.tgz