EVLA Continuum Tutorial 3C391: Difference between revisions

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[[Category:EVLA]][[Category:Calibration]]
== Overview ==
== Overview ==
This article describes the calibration and imaging of a multiple-pointing EVLA continuum dataset on the supernova remnant 3C 391. To generate the full data reduction script described here, use the [[Extracting_scripts_from_these_tutorials | script extractor]].
This article describes the calibration and imaging of a multiple-pointing EVLA continuum dataset on the supernova remnant 3C 391. The data were taken in OSRO1 mode, with 128 MHz of bandwidth in each of two widely spaced spectral windows, centered at 4.6 and 7.5 GHz, and were set up for full polarization calibration.  To generate the full data reduction script described here, use the [[Extracting_scripts_from_these_tutorials | script extractor]].
 
== Getting hold of your data ==
The data are publicly available from the [https://archive.nrao.edu/archive/archiveproject.jsp NRAO archive], under Project name TDEM0001.  The archive lists two separate files; one taken on 2010-Apr-15, and the other on 2010-Apr-24.  You will want to download the second file (file size 39.79 GB).  This file contains data at the full 1-s time resolution.

Revision as of 17:23, 4 May 2010


Overview

This article describes the calibration and imaging of a multiple-pointing EVLA continuum dataset on the supernova remnant 3C 391. The data were taken in OSRO1 mode, with 128 MHz of bandwidth in each of two widely spaced spectral windows, centered at 4.6 and 7.5 GHz, and were set up for full polarization calibration. To generate the full data reduction script described here, use the script extractor.

Getting hold of your data

The data are publicly available from the NRAO archive, under Project name TDEM0001. The archive lists two separate files; one taken on 2010-Apr-15, and the other on 2010-Apr-24. You will want to download the second file (file size 39.79 GB). This file contains data at the full 1-s time resolution.