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  • IRAS16293 Band9 - Imaging 6.4
    ...so need the [http://casaguides.nrao.edu/index.php?title=Analysis_Utilities Analysis Utils] package, so make sure you have it imported into CASA. ==Install Analysis Utilities==
    37 KB (5,507 words) - 14:15, 25 October 2022
  • IRAS16293 Band9 - Imaging for CASA 6.4
    ...so need the [http://casaguides.nrao.edu/index.php?title=Analysis_Utilities Analysis Utils] package, so make sure you have it imported into CASA. ==Install Analysis Utilities==
    37 KB (5,511 words) - 14:16, 25 October 2022
  • Self-Calibration Template CASA 6.1.1
    ...[https://casaguides.nrao.edu/index.php?title=Analysis_Utilities Obtaining Analysis Utilities] for instructions. Tasks such as {{plotants}} or {{listobs}}/{{vi
    21 KB (3,082 words) - 16:54, 28 February 2024
  • Simulating Observations in CASA 5.4
    ...sky model that was used for the analogous ALMA tutorial. Observational and analysis parameters are changed step by step and the results are compared to the VLA
    7 KB (1,016 words) - 12:22, 21 March 2024
  • Simulating Observations in CASA 6.5.4
    ...sky model that was used for the analogous ALMA tutorial. Observational and analysis parameters are changed step by step and the results are compared to the VLA
    6 KB (922 words) - 18:37, 26 March 2024
  • IRAS16293 Band9 - Imaging for CASA 6.5.4
    ...so need the [http://casaguides.nrao.edu/index.php?title=Analysis_Utilities Analysis Utils] package, so make sure you have it imported into CASA. ==Install Analysis Utilities==
    38 KB (5,651 words) - 08:54, 23 October 2023
  • Simulating Observations in CASA 6
    ...sky model that was used for the analogous ALMA tutorial. Observational and analysis parameters are changed step by step and the results are compared to the VLA
    7 KB (1,115 words) - 16:25, 12 February 2024
  • Sunspot Band6
    This guide has been split into four sections. '''For these tutorials, the [[Analysis Utilities]] package is required.'''
    6 KB (955 words) - 15:48, 16 April 2024
  • Measurement Set Contents
    ...ctions, but is also good information to keep in mind when performing basic analysis. For a complete description of the Measurement Set specifications, please
    8 KB (1,344 words) - 15:06, 9 August 2012
  • M100 Band3 SingleDish 5.1
    === Import "Analysis Utilities" === ...apping can be visualized by issuing the following command (after import of Analysis Utils - see the top of this page for information).
    39 KB (5,284 words) - 16:07, 19 August 2021
  • Sunspot Band6 Imaging for CASA 5.1
    Note: The FITS file can be imported to the data-analysis environment based on SolarSoftWare (SSW) + IDL without any modification, bu
    6 KB (1,016 words) - 16:37, 19 August 2021
  • M100 Band3 SingleDish 6.2
    === Import "Analysis Utilities" === ...apping can be visualized by issuing the following command (after import of Analysis Utils - see the top of this page for information).
    40 KB (5,491 words) - 11:39, 7 April 2022
  • M100 Band3 SingleDish 5.7
    === Import "Analysis Utilities" === ...apping can be visualized by issuing the following command (after import of Analysis Utils - see the top of this page for information).
    39 KB (5,356 words) - 14:36, 19 August 2021
  • M100 Band3 SingleDish 6.4
    === Import "Analysis Utilities" === ...apping can be visualized by issuing the following command (after import of Analysis Utils - see the top of this page for information).
    40 KB (5,491 words) - 11:06, 12 October 2023
  • M100 Band3 SingleDish 6.5.4
    === Import "Analysis Utilities" === ...apping can be visualized by issuing the following command (after import of Analysis Utils - see the top of this page for information).
    40 KB (5,472 words) - 16:52, 2 February 2024
  • M100 Band3 SingleDish 6.1
    === Import "Analysis Utilities" === ...apping can be visualized by issuing the following command (after import of Analysis Utils - see the top of this page for information).
    40 KB (5,435 words) - 14:37, 19 August 2021
  • M100 Band3 SingleDish 4.5
    === Import "Analysis Utilities" === ...apping can be visualized by issuing the following command (after import of Analysis Utils - see the top of this page for information).
    39 KB (5,283 words) - 01:21, 23 August 2017
  • PPdisk simdata (CASA 3.3)
    # The following command is used to open an image (this is part of the image analysis toolkit) |Analyze:<br> [[File:Psim2.analysis.png|300px]]
    6 KB (798 words) - 11:17, 22 November 2011
  • AntennaeBand7 North Imaging 3.4
    ...cy'''. Data are taken using constant frequency channels. For spectral line analysis it's often more useful to have constant velocity channels, and this is also ...output cube will also be in TOPO, which is not very useful for scientific analysis. The Doppler Shift is taken out during the regridding to the desired outfra
    40 KB (6,363 words) - 12:47, 5 June 2012
  • Simulating Observations in CASA 5.1
    ...sky model that was used for the analogous ALMA tutorial. Observational and analysis parameters are changed step by step and the results are compared to the VLA
    8 KB (1,252 words) - 17:23, 15 February 2023
  • Plotbandpass
    '''Return to [[Analysis Utilities]]''' This page documents the plotbandpass function of Python module [[Analysis Utilities|analysisUtils]].
    14 KB (2,237 words) - 13:13, 17 April 2024
  • EVLA high frequency Spectral Line tutorial - IRC+10216 part2 (Caltech)
    ==Image Analysis and Viewing== This analysis suggests that the rms noise on one baseline, one 10 second integration is a
    28 KB (4,570 words) - 17:09, 11 January 2012
  • EVLA high frequency Spectral Line tutorial - IRC+10216 part2
    ==Image Analysis and Viewing== This analysis suggests that the rms noise on one baseline, for one 10 second integration
    28 KB (4,647 words) - 20:37, 29 February 2012
  • EVLA high frequency Spectral Line tutorial - IRC+10216 part2-CASA3.3
    ==Image Analysis and Viewing== This analysis suggests that the rms noise on one baseline, for one 10 second integration
    28 KB (4,648 words) - 12:31, 9 April 2012
  • Imaging an EVLA OSRO HI data set
    == Other Analysis ==
    26 KB (3,652 words) - 12:22, 25 May 2010
  • 3C286 Polarization
    ...and6Pol_Imaging#Image_visualization_and_analysis | Image Visualization and Analysis]]''' section, where we also compare the results with available measurements
    7 KB (1,126 words) - 13:33, 18 October 2023
  • PythonBasics
    ...age of CASA's python shell to script your data reduction or integrate your analysis, observation planning, and reduction. Despite the CASA focus, we do aim to ...is functionality inside the interpreter, which is fantastic for rapid data analysis. Here we'll just look at the basics.
    34 KB (5,505 words) - 22:04, 6 March 2014
  • Antennae Band7 - Imaging for CASA 3.3
    ...cy'''. Data are taken using constant frequency channels. For spectral line analysis it's often more useful to have constant velocity channels, and this is also ...output cube will also be in TOPO, which is not very useful for scientific analysis. The Doppler Shift is taken out during the regridding to the desired outfra
    41 KB (6,416 words) - 16:05, 16 May 2012
  • M100 Band3 Combine 4.2.2
    == Image Analysis for the 7m+12m Data == Two functions in the analysis utilities suite can be used to calculate the sampling of the TP data in the
    37 KB (5,642 words) - 19:30, 19 May 2015
  • Sunspot Band6 Imaging for CASA 6.5.4
    Note: The FITS file can be imported to the data-analysis environment based on SolarSoftWare (SSW) + IDL without any modification, bu
    7 KB (1,154 words) - 14:35, 16 April 2024
  • IRAS16293 Band9 - Calibration for CASA 3.4
    ==Install Analysis Utilities== ...Utils for short) is a small set of Python scripts that provide a number of analysis and plotting utilities for ALMA data reduction. This guide uses a few of th
    66 KB (9,687 words) - 17:49, 15 June 2012
  • Sunspot Band6 Feathering for CASA 4.7
    ...rated data package ‘Sunspot_Band6_UncalibratedData.tgz’ and installing the Analysis Utilities package.
    9 KB (1,473 words) - 09:42, 11 January 2018
  • IRAS16293 Band9 - Calibration for CASA 4.0
    ==Install Analysis Utilities== ...Utils for short) is a small set of Python scripts that provide a number of analysis and plotting utilities for ALMA data reduction. This guide uses a few of th
    65 KB (9,635 words) - 13:24, 19 November 2012
  • Baseband Stitching
    ...et &mdash; see the [[EVLA Tutorials]] page for examples of calibration and analysis.
    11 KB (1,530 words) - 21:09, 1 March 2012
  • IRAS16293 Band9 - Calibration for CASA 4.1
    ==Install Analysis Utilities== ...Utils for short) is a small set of Python scripts that provide a number of analysis and plotting utilities for ALMA data reduction. This guide uses a few of th
    68 KB (10,006 words) - 21:13, 10 December 2013
  • 3C286 Band6Pol Imaging for CASA 4.3
    ==Image visualization and analysis==
    28 KB (4,145 words) - 09:41, 14 September 2017
  • 3C286 Band6Pol Imaging for CASA 4.5
    ==Image visualization and analysis==
    28 KB (4,149 words) - 09:48, 10 April 2017
  • Baseband Stitching-CASA4.1
    ...et &mdash; see the [[EVLA Tutorials]] page for examples of calibration and analysis.
    11 KB (1,581 words) - 13:47, 1 May 2013
  • AntennaeBand7 Imaging 3.4
    ...cy'''. Data are taken using constant frequency channels. For spectral line analysis it's often more useful to have constant velocity channels, and this is also ...output cube will also be in TOPO, which is not very useful for scientific analysis. The Doppler Shift is taken out during the regridding to the desired outfra
    44 KB (6,765 words) - 13:59, 11 October 2021
  • CARMA spectral line mosaic M99 3.1
    == Image Analysis == ...already have open (or reopen it if you closed it) to check the effect. For analysis that involves the true flux density like the moment 0, column density etc,
    37 KB (5,752 words) - 17:27, 26 May 2011
  • TWHydraBand7 Imaging 4.0
    ...cy'''. Data are taken using constant frequency channels. For spectral line analysis it's often more useful to have constant velocity channels, and this is also ==Image Analysis==
    62 KB (9,630 words) - 13:49, 19 December 2012
  • AntennaeBand7 Imaging 4.0
    ...cy'''. Data are taken using constant frequency channels. For spectral line analysis it's often more useful to have constant velocity channels, and this is also ...output cube will also be in TOPO, which is not very useful for scientific analysis. The Doppler Shift is taken out during the regridding to the desired outfra
    44 KB (6,844 words) - 15:05, 5 October 2021
  • AntennaeBand7 Imaging 4.4
    ...cy'''. Data are taken using constant frequency channels. For spectral line analysis it's often more useful to have constant velocity channels, and this is also ...output cube will also be in TOPO, which is not very useful for scientific analysis. The Doppler Shift is taken out during the regridding to the desired outfra
    44 KB (6,859 words) - 08:10, 5 October 2021
  • AntennaeBand7 Imaging 4.1
    ...cy'''. Data are taken using constant frequency channels. For spectral line analysis it's often more useful to have constant velocity channels, and this is also ...output cube will also be in TOPO, which is not very useful for scientific analysis. The Doppler Shift is taken out during the regridding to the desired outfra
    44 KB (6,858 words) - 10:48, 5 October 2021
  • AntennaeBand7 Imaging 4.2
    ...cy'''. Data are taken using constant frequency channels. For spectral line analysis it's often more useful to have constant velocity channels, and this is also ...output cube will also be in TOPO, which is not very useful for scientific analysis. The Doppler Shift is taken out during the regridding to the desired outfra
    44 KB (6,858 words) - 10:34, 5 October 2021
  • TWHydraBand7 Imaging 4.1
    ...cy'''. Data are taken using constant frequency channels. For spectral line analysis it's often more useful to have constant velocity channels, and this is also ==Image Analysis==
    63 KB (9,658 words) - 09:46, 18 June 2013
  • TWHydraBand7 Imaging 4.2
    ...cy'''. Data are taken using constant frequency channels. For spectral line analysis it's often more useful to have constant velocity channels, and this is also ==Image Analysis==
    63 KB (9,660 words) - 14:18, 12 November 2014
  • AntennaeBand7 Imaging 4.5
    ...cy'''. Data are taken using constant frequency channels. For spectral line analysis it's often more useful to have constant velocity channels, and this is also ...output cube will also be in TOPO, which is not very useful for scientific analysis. The Doppler Shift is taken out during the regridding to the desired outfra
    44 KB (6,883 words) - 07:26, 5 October 2021
  • AntennaeBand7 Imaging 4.3
    ...cy'''. Data are taken using constant frequency channels. For spectral line analysis it's often more useful to have constant velocity channels, and this is also ...output cube will also be in TOPO, which is not very useful for scientific analysis. The Doppler Shift is taken out during the regridding to the desired outfra
    44 KB (6,883 words) - 09:40, 5 October 2021
  • M100 Band3 SingleDish 4.3
    == Import "Analysis Utilities" == and the checkCalTable function of the Analysis Utilities.
    49 KB (6,272 words) - 16:27, 26 August 2015
  • IRAS16293 Band9 - Calibration for CASA 4.2
    ==Install Analysis Utilities== ...Utils for short) is a small set of Python scripts that provide a number of analysis and plotting utilities for ALMA data reduction. This guide uses a few of th
    68 KB (9,999 words) - 11:41, 12 November 2014
  • EVLA spectral line IRC10216
    * more on image analysis ==Image Analysis and Viewing==
    44 KB (6,777 words) - 12:19, 19 May 2010
  • CARMA spectral line mosaic M99 3.2
    == Image Analysis == ...already have open (or reopen it if you closed it) to check the effect. For analysis that involves the true flux density like the moment 0, column density etc,
    39 KB (6,041 words) - 13:04, 5 July 2011
  • TWHydraBand7 Imaging for CASA 3.3
    ...cy'''. Data are taken using constant frequency channels. For spectral line analysis it's often more useful to have constant velocity channels, and this is also ==Image Analysis==
    41 KB (6,493 words) - 21:20, 23 April 2012
  • TWHydraBand7 Imaging (Caltech)
    ...cy'''. Data are taken using constant frequency channels. For spectral line analysis it's often more useful to have constant velocity channels, and this is also ==Image Analysis==
    41 KB (6,495 words) - 18:36, 12 January 2012
  • ALMA Imaging Pipeline Reprocessing Tool
    - You can proceed with your scientific analysis starting with the uid*targets.ms files and supply them to CASA tasks such a
    12 KB (1,511 words) - 11:50, 20 October 2023
  • TWHydraBand7 Imaging 3.4
    ...cy'''. Data are taken using constant frequency channels. For spectral line analysis it's often more useful to have constant velocity channels, and this is also ==Image Analysis==
    45 KB (6,856 words) - 16:30, 12 June 2012
  • 3C286 Band6Pol Imaging for CASA 6.5.4
    ==Image visualization and analysis==
    30 KB (4,386 words) - 14:55, 23 October 2023
  • AntennaeBand7 Imaging 5.1
    For spectral line analysis it's often more useful to have constant velocity channels, and this is also ...output cube will also be in TOPO, which is not very useful for scientific analysis.
    47 KB (7,341 words) - 16:35, 20 August 2021
  • M100 Band3 Combine 4.5
    == Image Analysis for the 7m+12m Data == ...echnique as the [[#Moment_Maps_for_7m.2B12m_CO_.281-0.29_Cube|7m+12m image analysis above]] to make moment maps.
    37 KB (5,732 words) - 09:33, 10 April 2017
  • 3C286 Band6Pol Imaging for CASA 5.1
    ==Image visualization and analysis==
    32 KB (4,524 words) - 16:03, 3 April 2018
  • 3C286 Band6Pol Imaging for CASA 5.4
    ==Image visualization and analysis==
    31 KB (4,534 words) - 17:29, 11 March 2021
  • TWHydraBand7
    Cubes are available online for CO(2-1), CN(2-1), and CS(5-4) along with an analysis of the velocity dispersion from Teague et al. 2016.
    9 KB (1,372 words) - 22:05, 9 January 2017
  • 3C286 Band6Pol Imaging for CASA 5.7
    ==Image visualization and analysis==
    31 KB (4,537 words) - 17:31, 11 March 2021
  • 3C286 Band6Pol Imaging for CASA 6.1
    ==Image visualization and analysis==
    31 KB (4,537 words) - 09:10, 13 October 2021
  • 3C286 Band6Pol Imaging for CASA 6.2
    ==Image visualization and analysis==
    31 KB (4,537 words) - 10:20, 1 October 2021
  • EVLA Advanced Topics 3C391 CASA 4.2
    == Image Analysis and Manipulation == ...e can be found in [http://casa.nrao.edu/docs/UserMan/UserManch6.html Image Analysis] in the CASA Reference Book.
    46 KB (7,311 words) - 14:10, 6 February 2014
  • Advanced Topics 3C391 - CASA4.2
    == Image Analysis and Manipulation == ...e can be found in [http://casa.nrao.edu/docs/UserMan/UserManch6.html Image Analysis] in the CASA Reference Book.
    46 KB (7,311 words) - 13:51, 16 December 2014
  • AntennaeBand7 Imaging 5.4
    For spectral line analysis it's often more useful to have constant velocity channels, and this is also ...output cube will also be in TOPO, which is not very useful for scientific analysis.
    48 KB (7,478 words) - 15:24, 20 August 2021
  • AntennaeBand7 Imaging 5.7
    For spectral line analysis it's often more useful to have constant velocity channels, and this is also ...output cube will also be in TOPO, which is not very useful for scientific analysis.
    49 KB (7,485 words) - 15:44, 20 August 2021
  • AntennaeBand7 Imaging 6.1
    For spectral line analysis it's often more useful to have constant velocity channels, and this is also ...output cube will also be in TOPO, which is not very useful for scientific analysis.
    49 KB (7,492 words) - 13:22, 13 October 2021
  • AntennaeBand7 Imaging 6.2
    For spectral line analysis it's often more useful to have constant velocity channels, and this is also ...output cube will also be in TOPO, which is not very useful for scientific analysis.
    49 KB (7,524 words) - 11:23, 7 April 2022
  • AntennaeBand7 Imaging 6.4
    For spectral line analysis it's often more useful to have constant velocity channels, and this is also ...output cube will also be in TOPO, which is not very useful for scientific analysis.
    49 KB (7,509 words) - 00:55, 31 December 2023
  • Guide To Processing ALMA Data for Cycle 0
    # Generate moment maps and other analysis products ...o channels spaced by a constant frequency increment, but for spectral line analysis it's often more useful to have a constant velocity increment. For '''mode=
    46 KB (7,223 words) - 15:03, 7 September 2023
  • TwHydraBand7 Imaging SS12
    ...cy'''. Data are taken using constant frequency channels. For spectral line analysis it's often more useful to have constant velocity channels, and this is also ==Image Analysis==
    47 KB (7,259 words) - 16:08, 31 May 2012
  • EVLA Advanced Topics 3C391-CASA4.1
    == Image Analysis and Manipulation == ...e can be found in [http://casa.nrao.edu/docs/UserMan/UserManch6.html Image Analysis] in the CASA Reference Book.
    47 KB (7,334 words) - 19:42, 4 February 2014
  • Advanced Topics 3C391 - CASA4.1
    == Image Analysis and Manipulation == ...e can be found in [http://casa.nrao.edu/docs/UserMan/UserManch6.html Image Analysis] in the CASA Reference Book.
    47 KB (7,335 words) - 19:50, 4 February 2014
  • EVLA Advanced Topics 3C391
    == Image Analysis and Manipulation == ...e can be found in [http://casa.nrao.edu/docs/UserMan/UserManch6.html Image Analysis] in the CASA Reference Book.
    47 KB (7,549 words) - 16:36, 20 April 2015
  • EVLA Advanced Topics 3C391-CASA4.3
    == Image Analysis and Manipulation == ...e can be found in [http://casa.nrao.edu/docs/UserMan/UserManch6.html Image Analysis] in the CASA Reference Book.
    47 KB (7,549 words) - 16:32, 20 April 2015
  • EVLA Advanced Topics 3C391-CASA4.4
    == Image Analysis and Manipulation == ...e can be found in [http://casa.nrao.edu/docs/UserMan/UserManch6.html Image Analysis] in the CASA Reference Book.
    47 KB (7,551 words) - 13:47, 2 June 2015
  • EVLA Advanced Topics 3C391-CASA4.0
    == Image Analysis and Manipulation == ...e can be found in [http://casa.nrao.edu/docs/UserMan/UserManch6.html Image Analysis] in the CASA Reference Book.
    47 KB (7,436 words) - 16:17, 30 May 2013
  • EVLA Advanced Topics 3C391-CASA3.4
    == Image Analysis and Manipulation == ...d in [http://casa.nrao.edu/docs/userman/UserManch6.html#x310-3050006 Image Analysis] in the CASA Reference Book.
    47 KB (7,454 words) - 17:12, 22 October 2012
  • Protoplanetary Disk Simulation - VLA-CASA6.4.1
    ...AO replacement visualization tool for images and cubes is CARTA, the “Cube Analysis and Rendering Tool for Astronomy”. It is available from the [https://cart ...api/tt/casatasks.simulation.simobserve.html simobserve] will perform basic analysis of the generated images and create hard copies of the following displays.
    45 KB (6,774 words) - 15:57, 27 January 2023
  • IRAS16293 Band9 - Calibration for CASA 4.3
    ==Install Analysis Utilities== ...Utils for short) is a small set of Python scripts that provide a number of analysis and plotting utilities for ALMA data reduction. This guide uses a few of th
    68 KB (9,999 words) - 13:32, 12 September 2017
  • IRAS16293 Band9 - Calibration for CASA 4.5
    ==Install Analysis Utilities== ...Utils for short) is a small set of Python scripts that provide a number of analysis and plotting utilities for ALMA data reduction. This guide uses a few of th
    68 KB (10,027 words) - 13:15, 4 April 2017
  • IRAS16293 Band9 - Calibration for CASA 4.4
    ==Install Analysis Utilities== ...Utils for short) is a small set of Python scripts that provide a number of analysis and plotting utilities for ALMA data reduction. This guide uses a few of th
    68 KB (9,999 words) - 21:50, 6 July 2015
  • TWHydraBand7 Calibration 3.4
    ==Install Analysis Utilities== ...Utils for short) is a small set of Python scripts that provide a number of analysis and plotting utilities for ALMA data reduction. This guide uses a few of th
    76 KB (11,820 words) - 10:34, 25 July 2012
  • TWHydraBand7 Imaging 4.4
    ...cy'''. Data are taken using constant frequency channels. For spectral line analysis it's often more useful to have constant velocity channels, and this is also ==Image Analysis==
    63 KB (9,660 words) - 21:36, 6 July 2015
  • Protoplanetary Disk Simulation - VLA-CASA6.5.4
    ...AO replacement visualization tool for images and cubes is CARTA, the “Cube Analysis and Rendering Tool for Astronomy”. It is available from the [https://cart ...api/tt/casatasks.simulation.simobserve.html simobserve] will perform basic analysis of the generated images and create hard copies of the following displays.
    46 KB (6,895 words) - 14:39, 28 February 2024
  • TWHydraBand7 Imaging 4.3
    ...cy'''. Data are taken using constant frequency channels. For spectral line analysis it's often more useful to have constant velocity channels, and this is also ==Image Analysis==
    62 KB (9,547 words) - 17:00, 19 August 2021
  • IRAS16293 Band9 Calibration
    ==Install Analysis Utilities== ...Utils for short) is a small set of Python scripts that provide a number of analysis and plotting utilities for ALMA data reduction. This guide uses a few of th
    69 KB (10,222 words) - 15:51, 12 September 2017
  • TWHydraBand7 Calibration 4.1
    ==Install Analysis Utilities== ...Utils for short) is a small set of Python scripts that provide a number of analysis and plotting utilities for ALMA data reduction. This guide uses a few of th
    78 KB (12,026 words) - 21:09, 10 December 2013
  • M100 Band3 Combine 5.7
    == Image Analysis for the 7m+12m Data == ...echnique as the [[#Moment_Maps_for_7m.2B12m_CO_.281-0.29_Cube|7m+12m image analysis above]] to make moment maps.
    39 KB (5,971 words) - 14:39, 19 August 2021
  • TWHydraBand7 Calibration 4.0
    ==Install Analysis Utilities== ...Utils for short) is a small set of Python scripts that provide a number of analysis and plotting utilities for ALMA data reduction. This guide uses a few of th
    78 KB (12,045 words) - 16:58, 7 November 2012
  • EVLA high frequency Spectral Line tutorial - IRC+10216 part1 (Caltech)
    ....nrao.edu/opportunities/courses/casa-caltech-winter2012 Caltech CASA Radio Analysis Workshop] or are doing the tutorial on your own. === At the Caltech CASA Radio Analysis Workshop ===
    53 KB (8,284 words) - 01:44, 19 January 2012
  • AntennaeBand7 Imaging 6.5.4
    For spectral line analysis it's often more useful to have constant velocity channels, and this is also ...output cube will also be in TOPO, which is not very useful for scientific analysis.
    51 KB (7,819 words) - 15:29, 29 February 2024
  • OtherPackages
    ...y rise to the level of inclusion but all are super useful for post-imaging analysis.
    12 KB (1,972 words) - 17:59, 9 July 2019
  • M100 Band3 Combine 5.4
    == Image Analysis for the 7m+12m Data == ...echnique as the [[#Moment_Maps_for_7m.2B12m_CO_.281-0.29_Cube|7m+12m image analysis above]] to make moment maps.
    40 KB (6,024 words) - 16:09, 19 August 2021
  • M100 Band3 Combine 6.1
    == Image Analysis for the 7m+12m Data == ...echnique as the [[#Moment_Maps_for_7m.2B12m_CO_.281-0.29_Cube|7m+12m image analysis above]] to make moment maps.
    40 KB (6,039 words) - 14:44, 19 August 2021
  • M100 Band3 Combine 6.2
    == Image Analysis for the 7m+12m Data == ...echnique as the [[#Moment_Maps_for_7m.2B12m_CO_.281-0.29_Cube|7m+12m image analysis above]] to make moment maps.
    40 KB (6,067 words) - 11:49, 7 April 2022

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