ALMA Tutorials draft

Introduction

This page contains tutorials to guide ALMA users through some common types of data imaging and analysis using CASA with example ALMA datasets. Here are some links to get started:

	ALMA Science homepage
	CASA homepage: includes download and installation information CASA Docs CASA Tips Getting Started in CASA How To Use A CASAGuide Extracting scripts from these tutorials To cite CASA, please use: \bibitem[CASA Team et al.(2022)]{2022PASP..134k4501C} CASA Team, Bean, B., Bhatnagar, S., et al.\ 2022, PASP, 134, 114501. doi:10.1088/1538-3873/ac9642
File:Pipeline logo.png	ALMA Pipeline webpage ALMA Pipeline Known Issues To cite the ALMA pipeline, please use: \bibitem[Hunter et al.(2023)]{2023PASP..135g4501H} Hunter, T.~R., Indebetouw, R., Brogan, C.~L., et al.\ 2023, PASP, 135, 074501. doi:10.1088/1538-3873/ace216
	CARTA website CARTA section of the CASA docs

Basic Imaging and Analysis

ALMA data are delivered to users with calibrations applied and they are ready for imaging. The following "First Look" tutorials provide short examples of common next steps a user may take with their calibrated data. These guides use an example ALMA observation of TW Hydra.

First Look at Imaging (continuum)	This is a really long sentence to force the table to fill the full page width otherwise it looks bad. This is a really long sentence to force the table to fill the full page width otherwise it looks bad.	File:TWHya.png
First Look at Self Calibration	description
First Look at Line Imaging	description
First Look at Image Analysis	description

Older versions of these guides are archived here: ALMA First Look

Advanced Imaging

Modified Pipeline Imaging
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Manual Imaging Templates
description
Automasking
description
Jump to special imaging topics from the End to End guides:
AntennaeBand7 > Mosaic Imaging IRAS16293 Band9 > Mosaic Imaging M100 Band3 > Image Combination 3C286 Band6 > Full Polarization Imaging Sunspot Band6 > Image Combination

End to End Guides (Manual Calibration)

These guides are useful tools for those who would like to learn the process of calibration and imaging in detail. They use publicly-available ALMA Science Verification data that illustrate several different ALMA capabilities. The links below lead to overview pages for each observation. The guides themselves are linked from the overview pages.

AntennaeBand7
This is a really long sentence to force the table to fill the full page width otherwise it looks bad. This is a really long sentence to force the table to fill the full page width otherwise it looks bad. Band 7 (345 GHz, 0.87 mm) CO 3-2 spectral line Antennae Galaxy Merger (NGC 4038/4039) North and South mosaics
IRAS16293Band9
Band 9 (650 GHz, 0.46 mm) Protostellar Cluster High frequency techniques Mosaic
M100 Band3
Band 3 (100 GHz, 3 mm) on M100 demonstrates Single Dish (Total Power) data reduction and 12m , 7m, Total Power combination procedures.
3C286 Polarization
Band 6 (230 GHz, 1.3 mm) Continuum polarization calibration and imaging
Sunspot Band6
Band 6 (230 GHz, 1.3 mm) Solar observing techniques Calibration and imaging Helper scripts

Special Topics

• Renormalization
• Data Weights

- relevant for data from Cycles 0, 1, and 2

• Simulating Observations

- Also see: Guide To Simulating ALMA Data

Legacy Guides

• Archived ALMA CASAguides
• TCLEAN and ALMA

• Cycle 0

- Last checked in CASA 4.2

- Helpful hints for downloading the data

- Imaging, self-calibration, and image analysis

Example data calibration scripts used for Cycle 0 data (CASA 3.4):

• File:TDM.example.ms.scriptForCalibration.py: TDM (128 channels/spw)
• File:FDM.example.ms.scriptForCalibration.py: FDM (3840 channels/spw)
• Updating a script to work with CASA 4.2: Update 3.4 scripts to 4.2 or later.

Resources

• ALMA Sensitivity Calculator
• ADMIT Products and Usage: This guide discusses how to use the ALMA Data-Mining Toolkit (ADMIT) and customize it for your data.
• Analysis Utilities: A Python module containing utilities for analysis and plotting.
• Karl G. Jansky VLA Tutorials
• Past MM/Submm Guides: These are not currently being maintained.