ALMA Tutorials draft: Difference between revisions

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* [[ALMA Renormalization Correction | Renormalization]]  
* [[ALMA Renormalization Correction | Renormalization]]  
* [[DataWeightsAndCombination | Data Weights]]  
* [[DataWeightsAndCombination | Data Weights]]  
* [[Guide To Simulating ALMA Data]]
:- relevant for data from Cycles 0, 1, and 2
* [[Simulating Observations in CASA | Simulation]]
* [[Simulating Observations in CASA | Simulating Observations]]
:- Also see: [[Guide To Simulating ALMA Data]]


== End to End Guides (Manual Calibration) ==
== End to End Guides (Manual Calibration) ==

Revision as of 20:38, 7 October 2024

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
CASA
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

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

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.

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

Advanced Imaging

The following are the portions of the End to End guides that cover special imaging topics. The full End to End guides with manual calibration are listed further down this page:

Special Topics

- relevant for data from Cycles 0, 1, and 2
- Also see: Guide To Simulating ALMA Data

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

  • 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)
  • Total Power (Single Dish) calibration and imaging
  • Combining 12m-array, 7m-array, and Total Power data

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

Legacy Guides

- 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):

Resources

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