ALMAguides: Difference between revisions
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* <font size = 3>'''ALMA Science Verification | * <font size = 3>'''Guides for reducing ALMA Science Verification data using CASA 4.2'''</font size> | ||
** The links below lead to overview pages for each science | ** The links below lead to overview pages for each science verification observation. The guides themselves are linked from the overview pages. These guides are a useful tools for those who would like to learn the process of calibration and imaging in detail. | ||
** [[TWHydraBand7 | TWHydraBand7]]: The protoplanetary disk source TW Hya at Band 7 (0.87 mm) | ** [[TWHydraBand7 | TWHydraBand7]]: The protoplanetary disk source TW Hya at Band 7 (0.87 mm) | ||
** [[NGC3256Band3 | NGC3256Band3]]: The galaxy merger NGC 3256 at Band 3 (3 mm) | ** [[NGC3256Band3 | NGC3256Band3]]: The galaxy merger NGC 3256 at Band 3 (3 mm) | ||
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[[IRAS16293_Band9_-_Imaging_for_CASA_4.1]] | [[IRAS16293_Band9_-_Imaging_for_CASA_4.1]] | ||
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* <font size = 3>'''[[Guide_To_Processing_ALMA_Data_for_Cycle_0 | A Guide to Processing ALMA Data for Cycle 0]]'''</font size> | |||
** This page takes you through the steps of processing Cycle 0 data from the ALMA data archive. The guide describes some helpful hints for downloading the data, and describes the process all the way through imaging and self-calibration, and image analysis. | |||
** You can also get a look at example data calibration scripts used for Cycle 0 data at the following links. These were written for CASA 3.4 The latest version is 4.2. | |||
*** TDM (128 channels/spw) [[File:TDM.example.ms.scriptForCalibration.py]] | |||
*** FDM (3840 channels/spw) [[File:FDM.example.ms.scriptForCalibration.py]] | |||
*** If you need to update 3.4 scripts to 4.2, see more information [[Updating_a_script_to_work_with_CASA_4.2|here]] | |||
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* <font size = 3>'''[[Analysis Utilities]] -- a Python module containing utilities for analysis and plotting.'''</font size> | * <font size = 3>'''[[Analysis Utilities]] -- a Python module containing utilities for analysis and plotting.'''</font size> | ||
Revision as of 10:34, 16 April 2014
- Guides for reducing ALMA Science Verification data using CASA 4.2
- The links below lead to overview pages for each science verification observation. The guides themselves are linked from the overview pages. These guides are a useful tools for those who would like to learn the process of calibration and imaging in detail.
- TWHydraBand7: The protoplanetary disk source TW Hya at Band 7 (0.87 mm)
- NGC3256Band3: The galaxy merger NGC 3256 at Band 3 (3 mm)
- AntennaeBand7: Mosaic of the galaxy merger NGC 4038/4039 (Antennae) at Band 7 (0.87 mm)
- IRAS16293Band9: Mosaic of the protostellar cluster IRAS16293-2422 at Band 9 (0.45 mm)
- File:BR1202 SV Band7 Calibration notes.pdf: Supplemental notes on the calibration of Science Verification target BR1202-0725 in CASA 3.3
- A Guide to Processing ALMA Data for Cycle 0
- This page takes you through the steps of processing Cycle 0 data from the ALMA data archive. The guide describes some helpful hints for downloading the data, and describes the process all the way through imaging and self-calibration, and image analysis.
- You can also get a look at example data calibration scripts used for Cycle 0 data at the following links. These were written for CASA 3.4 The latest version is 4.2.
- TDM (128 channels/spw) File:TDM.example.ms.scriptForCalibration.py
- FDM (3840 channels/spw) File:FDM.example.ms.scriptForCalibration.py
- If you need to update 3.4 scripts to 4.2, see more information here
- A Guide to Simulating ALMA Data. Start here to learn about simulations.
- Jump directly to the simulations examples with the following links. Current version = 4.2
- Analysis Utilities -- a Python module containing utilities for analysis and plotting.
- Solar System Models in CASA 4.0 and beyond
- Other useful Information
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