Guide to the NA Imaging Template: Difference between revisions

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== About this Guide ==
== About this Guide ==


This guide describes the template script used to manually image data for quality assurance by the North America ALMA Science Center (NAASC). This script is designed to guide the user through the decisions needed when imaging ALMA data. It should not be applied blindly; not all sections of the template imaging scripts are relevant for all data sets.  See the [[ALMA_Imaging_Pipeline_Reprocessing | ALMA Imaging Pipeline Reprocessing]] guide for information on pipeline processed images.
This guide describes the template script used to manually image data for quality assurance by the North America ALMA Science Center (NAASC). This script is designed to guide the user through the decisions needed when imaging ALMA data. It should not be applied blindly; not all sections of the template imaging scripts are relevant for all data sets. It can be adapted for pipeline processed images by the user.  See the [[ALMA_Imaging_Pipeline_Reprocessing | ALMA Imaging Pipeline Reprocessing]] guide for information on pipeline processed images.
All example images were produced using ALMA Science Verification Data of TW Hya. More information along with the dataset can be obtained from the [https://casaguides.nrao.edu/index.php/TWHydraBand7 TW Hydra Band 7 Calibration and Imaging Guide].
All example images were produced using ALMA Science Verification Data of TW Hya. More information along with the dataset can be obtained from the [https://casaguides.nrao.edu/index.php/TWHydraBand7 TW Hydra Band 7 Calibration and Imaging Guide].

Revision as of 13:24, 6 May 2017

About this Guide

This guide describes the template script used to manually image data for quality assurance by the North America ALMA Science Center (NAASC). This script is designed to guide the user through the decisions needed when imaging ALMA data. It should not be applied blindly; not all sections of the template imaging scripts are relevant for all data sets. It can be adapted for pipeline processed images by the user. See the ALMA Imaging Pipeline Reprocessing guide for information on pipeline processed images.

All example images were produced using ALMA Science Verification Data of TW Hya. More information along with the dataset can be obtained from the TW Hydra Band 7 Calibration and Imaging Guide.

A current version of the script can be found on github. A description of how the script is used at the NAASC can be found in Kepley et al. Proceedings of the SPIE, 9910, 99100C

Prepare for Imaging

Before you begin imaging, it is important to determine whether the data is manually or pipeline calibrated. The README file should state how the dataset was calibrated. If it does not, look in the script directory of the delivered data package. If you see a file named <ASDM UID>.ms.scriptForCalibration.py, the dataset was manually calibrated. If you see a filename PPR_*.xml, the dataset was pipeline calibrated.

We recommended that you use the same version of CASA for imaging as which the original reduction was performed. [xxx IS THIS REALLY TRUE? AFTER 4.2 THE WEIGHTS ISSUE SHOULD BE OKAY. I WOULD DOWNGRADE THIS OR ADD SOME SPECIFICS.] Refer to the README file or CASA logs to see which version was used. Download CASA and check for operating system requirements before proceeding.

Instructions on restoring the calibrated measurement set should be found in the README of your delivered dataset. For most cases, this can be done by executing scriptForPI.py in CASA in the script directory.

# in CASA
execfile(scriptForPI.py)

Attached Scripts

Two template scripts are available for this guide. These contain commands with minimal instructions and are intended to be used by those more familiar with imaging.

Obtaining Analysis Utilities

Some optional steps in this guide use the Analysis Utilities package. If you wish to use any of these tasks, follow the link above for download and installation instructions.

CASA and Interferometry Basics

If you are new to interferometry or CASA, we recommend you follow the “First Look” Imaging Tutorials. The Synthesis Imaging Summer School Lectures provide a wealth of information on interferometry.

In addition, many frequently asked questions can be found in the ALMA Knowledgebase. If you have additional questions after reviewing this guide, please contact the ALMA Helpdesk.

Guides for Using the North American ALMA Manual Imaging Template

This guide has been split into 4 sections:

  1. Prepare the data for Imaging This page creates the calibrated_final.ms that will be used in during imaging. Commands can be found in scriptForImagingPrep_template.py attached to this page.
  2. Image the Continuum Template This page creates a continuum measurement set (MS) and continuum images. The MS created in Imaging_Prep is needed for this guide. Commands can be found in scriptForImaging.py attached to this page.
  3. Self-Calibration Template This page provides a basic template for phase and amplitude self calibration of the continuum. The MS created in Image_Continuum is needed for this guide. Commands can be found in scriptForImaging.py attached to this page.
  4. Spectral Line Imaging Template This page performs continuum subtraction and creates spectral line cubes. The MS created in Imaging_Prep is needed for this guide. Commands can be found in scriptForImaging.py attached to this page.

The Imaging Workflow gives an outline of possible imaging you may do with the above guides.

How to Use A CASA Guide

For tips on using CASA and ways CASA can be run, see EVLA_Spectral_Line_Calibration_IRC+10216#How_to_Use_This_casaguide page.

To learn how to extract executable Python scripts from the tutorial, see Extracting_scripts_from_these_tutorials.

Within the guides:

# In CASA
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# Tabs matter in python, make sure that commands that span more than one line and 
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# explicitly hit enter twice to get the command going.
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