Search results

• EVLA high frequency Spectral Line tutorial - IRC+10216-newfile
  ==Image Analysis and Viewing== This analysis suggests that the rms noise on one baseline, for one 10 second integration
  83 KB (13,039 words) - 18:00, 20 July 2015
• VLA Polarization pipe Tutorial
  ...ant to convert the Stokes images into something more useful for scientific analysis. We will use CASA to calculate polarization intensity, <math>\sqrt{Q^2 + U^ ...The fits using [https://casadocs.readthedocs.io/en/v6.4.1/api/tt/casatasks.analysis.rmfit.html rmfit] for our case of 3C 75 by making images per spectral windo
  123 KB (17,782 words) - 13:42, 22 April 2024
• VLA Continuum Intro Tutorial
  ...NRAO replacement visualization tool for images and cubes, CARTA the “Cube Analysis and Rendering Tool for Astronomy”. It is available from the [https://cart == Image Analysis ==
  124 KB (19,294 words) - 17:49, 14 May 2024
• Jupiter: continuum polarization calibration 5.5.0
  And that's it. For the tutorial on how to perform analysis, display and manipulation of the polarisation images now, consult the appro
  25 KB (3,544 words) - 13:00, 13 February 2023
• EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.5
  ==Image Analysis and Viewing== This analysis suggests that the rms noise on one baseline, for one 10 second integration,
  90 KB (14,142 words) - 18:38, 10 March 2016
• VLA high frequency Spectral Line tutorial - IRC+10216-CASA5.5.0
  ==Image Analysis and Viewing== ...ssion is described in the [[Masking_images_for_analysis|Masking Images for Analysis]] page.
  108 KB (16,739 words) - 15:08, 15 October 2020
• VLA high frequency Spectral Line tutorial - IRC+10216-CASA4.7
  ==Image Analysis and Viewing== This analysis suggests that the rms noise on one baseline, for one 10 second integration,
  92 KB (14,512 words) - 17:26, 25 May 2017
• VLA high frequency Spectral Line tutorial - IRC+10216-CASA5.7.0
  ==Image Analysis and Viewing== ...ssion is described in the [[Masking_images_for_analysis|Masking Images for Analysis]] page.
  108 KB (16,776 words) - 15:14, 15 October 2020
• VLA high frequency Spectral Line tutorial - IRC+10216-CASA4.6
  ==Image Analysis and Viewing== This analysis suggests that the rms noise on one baseline, for one 10 second integration,
  92 KB (14,496 words) - 16:50, 7 November 2016
• VLA Self-calibration Tutorial-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 ...ation procedure. This is also what was chosen for the scientific image and analysis because the artifacts from the outlying sources did not strongly effect the
  91 KB (13,780 words) - 12:03, 2 April 2024
• VLA high frequency Spectral Line tutorial - IRC+10216-CASA6.2.0
  ==Image Analysis and Viewing== ...eadthedocs.io/en/v6.2.0/api/tt/casatasks.analysis.immoments.html#casatasks.analysis.immoments immoments]'''. In order to do this, we will want to know what cha
  119 KB (18,324 words) - 12:17, 24 February 2023
• VLA high frequency Spectral Line tutorial - IRC+10216-CASA6.4.1
  ==Image Analysis and Viewing== ...eadthedocs.io/en/v6.2.0/api/tt/casatasks.analysis.immoments.html#casatasks.analysis.immoments immoments]'''. In order to do this, we will want to know what cha
  119 KB (18,324 words) - 14:03, 2 March 2023
• EVLA 3-bit Tutorial G192-CASA4.3
  In addition, only the fields used for analysis and observation are included in the downloadable file. This can be accompl # In CASA: splitting fields for analysis
  155 KB (16,800 words) - 23:15, 4 June 2015
• EVLA 3-bit Tutorial G192-CASA4.4
  In addition, only the fields used for analysis and observation are included in the downloadable file. This can be accompl # In CASA: splitting fields for analysis
  155 KB (16,783 words) - 15:49, 13 April 2016
• VLA high frequency Spectral Line tutorial - IRC+10216-CASA5.0.0
  ==Image Analysis and Viewing== This analysis suggests that the rms noise on one baseline, for one 10 second integration,
  98 KB (15,214 words) - 11:44, 3 October 2018
• VLA Data Combination-W49A-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 CARTA website
  30 KB (3,840 words) - 17:11, 22 February 2024
• VLA Data Combination-W49A-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 CARTA website
  30 KB (3,847 words) - 16:55, 22 February 2024
• Polarization Calibration based on CASA pipeline standard reduction: The radio galaxy 3C75-CASA5.4.2
  ...ant to convert the Stokes images into something more useful for scientific analysis. We will use the CASA to calculate polarization intensity (sqrt(Q^2 + U^2)/ <!-- == Image Analysis ==
  131 KB (17,960 words) - 19:34, 20 November 2019
• VLA high frequency Spectral Line tutorial - IRC+10216-CASA5.4.0
  ==Image Analysis and Viewing== This analysis suggests that the rms noise on one baseline, for one 10 second integration,
  108 KB (16,694 words) - 10:46, 11 June 2019
• VLA CASA Imaging-CASA6.5.2
  ...ing '''T'''ool for '''A'''stronomy, a new tool for image visualization and analysis developed for the VLA, ALMA, and future radio telescopes. CASA is no longer ...s.readthedocs.io/en/v6.5.2/api/tt/casatasks.analysis.immath.html#casatasks.analysis.immath immath] to manually divide the ''<imagename>.image'' by the ''<image
  75 KB (11,832 words) - 14:03, 7 February 2023
• MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.2
  ...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 ...and, we only use a small fraction of the total band for data reduction and analysis in this tutorial.
  66 KB (9,867 words) - 13:55, 24 January 2024
• MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.4 MG0414 0534 P-band Spectral Line Tutorial (CASA 6.5.4)
  ...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 ...and, we only use a small fraction of the total band for data reduction and analysis in this tutorial.
  66 KB (9,882 words) - 11:21, 29 February 2024
• MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.4
  ...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 ...and, we only use a small fraction of the total band for data reduction and analysis in this tutorial.
  66 KB (9,882 words) - 14:06, 29 February 2024
• VLA CASA Imaging-CASA6.5.4
  ...ing '''T'''ool for '''A'''stronomy, a new tool for image visualization and analysis developed for the VLA, ALMA, and future radio telescopes. CASA is no longer ...s.readthedocs.io/en/v6.5.4/api/tt/casatasks.analysis.immath.html#casatasks.analysis.immath immath] to manually divide the ''<imagename>.image'' by the ''<image
  77 KB (12,054 words) - 13:56, 1 March 2024
• VLA Continuum Tutorial 3C391-CASA6.4.1
  ...NRAO replacement visualization tool for images and cubes, CARTA the “Cube Analysis and Rendering Tool for Astronomy”. It is available from the [https://cart == Image Analysis ==
  154 KB (22,682 words) - 12:13, 1 March 2024
• AntennaeBand7 North Calibration 3.4
  ...ve verified that you have the right version of CASA and have access to the analysis utilities module, you can are ready to begin. We loop through and using analysis utils, again generating .png files of each calibration. As the bandpass plo
  101 KB (15,763 words) - 13:48, 5 June 2012
• Protoplanetary Disk Simulation - VLA-CASA5.3.0
  '''analyze:''' When set to ''True'' {{simobserve}} will perform basic analysis of the produced images and produce hard copies of the following displays.
  36 KB (5,572 words) - 16:38, 30 October 2018
• VLA high frequency Spectral Line tutorial - IRC+10216-CASA6.5.3
  ...hen looking through archival or unfamiliar data. To simplify the following analysis, we will assign these names to Python variables for re-use with different t ...flagging.flagdata flagdata]''' to flag the data to exclude it from further analysis and calibration:
  134 KB (19,330 words) - 16:53, 29 September 2023
• EVLA 3-bit Tutorial G192 - CASA4.1
  In addition, only the fields used for analysis and observation are included in the downloadable file. This can be accompl ...would need to go through a more thorough investigation of the actual error analysis and spectral index.
  136 KB (14,700 words) - 19:55, 4 February 2014
• Protoplanetary Disk Simulation - VLA-CASA5.4.0
  '''analyze:''' When set to ''True'', {{simobserve}} will perform basic analysis of the generated images and create hard copies of the following displays.
  39 KB (5,805 words) - 14:55, 19 March 2019
• VLA Continuum Tutorial 3C391-CASA5.5.0
  == Image Analysis == ...e found in the [https://casa.nrao.edu/casadocs/latest/image-analysis Image Analysis] section of the CASA documentation.
  142 KB (20,826 words) - 13:06, 14 July 2020
• VLA Continuum Tutorial 3C391-CASA5.7.0
  == Image Analysis == ...e found in the [https://casa.nrao.edu/casadocs/latest/image-analysis Image Analysis] section of the CASA documentation.
  144 KB (21,056 words) - 15:58, 29 October 2020
• VLA 5 GHz continuum survey of Seyfert galaxies 6.4.1
  ...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
  34 KB (5,086 words) - 17:13, 3 February 2023
• VLA Continuum Tutorial 3C391-CASA6.2.0
  == Image Analysis == ...ps://casadocs.readthedocs.io/en/v6.2.0/notebooks/image_analysis.html Image Analysis] section of the CASA documentation.
  153 KB (22,510 words) - 11:29, 14 February 2023
• MRK 6: red-shifted HI absorption 6.5.2
  ...AO replacement visualization tool for images and cubes is CARTA, the “Cube Analysis and Rendering Tool for Astronomy”. It is available from the CARTA website ...mstat imstat], [https://casadocs.readthedocs.io/en/v6.5.2/api/tt/casatasks.analysis.imval.html imval], and [https://casadocs.readthedocs.io/en/v6.5.2/api/tt/ca
  35 KB (5,087 words) - 17:54, 8 February 2023
• VLA Continuum Tutorial 3C391-CASA5.4.0
  == Image Analysis == ...e found in the [https://casa.nrao.edu/casadocs/latest/image-analysis Image Analysis] section of the CASA documentation.
  145 KB (21,313 words) - 19:35, 2 January 2019
• VLA CASA Pipeline-full-CASA4.7.2
  ...ven on [https://casaguides.nrao.edu/index.php?title=Analysis_Utilities the Analysis Utils CASAguides page]. The functions to change scan intents are ''au.editI
  85 KB (13,006 words) - 18:57, 19 May 2017
• EVLA Continuum Tutorial 3C391-CASA3.4
  ....php?title=EVLA_Advanced_Topics_3C391-CASA3.4 3C391 Tutorial Part 2: Image Analysis, Polarization, Self-calibration] which follows on from this one. ...ill carry out the polarization imaging, self-calibration, and polarization analysis and display of the data.
  116 KB (17,150 words) - 17:11, 22 October 2012
• EVLA Continuum Tutorial 3C391-CASA4.0
  ...du/index.php?title=EVLA_Advanced_Topics_3C391 3C391 Tutorial Part 2: Image Analysis, Polarization, Self-calibration] which follows on from this one. ...ill carry out the polarization imaging, self-calibration, and polarization analysis and display of the data.
  117 KB (17,075 words) - 16:16, 30 May 2013
• VLA Self-calibration Tutorial-CASA5.7.0
  ...ation procedure. This is also what was chosen for the scientific image and analysis because the artifacts from the outlying sources did not strongly effect the ...have been reduced to a level that is no longer problematic for scientific analysis of the central source. This is primarily the result of improving phase cali
  86 KB (13,200 words) - 15:40, 18 October 2020
• EVLA 3-bit Tutorial G192-CASA4.2
  In addition, only the fields used for analysis and observation are included in the downloadable file. This can be accompl ...would need to go through a more thorough investigation of the actual error analysis and spectral index.
  155 KB (16,512 words) - 00:59, 5 February 2014
• VLA Self-calibration Tutorial-CASA6.2.0
  ...ation procedure. This is also what was chosen for the scientific image and analysis because the artifacts from the outlying sources did not strongly effect the ...have been reduced to a level that is no longer problematic for scientific analysis of the central source. This is primarily the result of improving phase cali
  94 KB (14,384 words) - 17:33, 20 July 2021
• EVLA 6-cm Wideband Tutorial SN2010FZ
  ...te to identify the frequency/channel of RFI. In particular, we note in our analysis: the same for this final image. Here, we will do some rough analysis on the spectral index to determine
  93 KB (12,148 words) - 18:33, 27 January 2012
• EVLA Continuum Tutorial 3C391-CASA3.3
  ....php?title=EVLA_Advanced_Topics_3C391-CASA3.3 3C391 Tutorial Part 2: Image Analysis, Polarization, Self-calibration] ....php?title=EVLA_Advanced_Topics_3C391-CASA3.3 3C391 Tutorial Part 2: Image Analysis, Polarization, Self-calibration]
  94 KB (13,931 words) - 12:32, 9 April 2012
• EVLA 6cmWideband Tutorial SN2010FZ-CASA3.3
  ...te to identify the frequency/channel of RFI. In particular, we note in our analysis: the same for this final image. Here, we will do some rough analysis on the spectral index to determine
  95 KB (12,507 words) - 11:51, 23 May 2012
• EVLA Continuum Tutorial 3C391 - CASA 4.1
  ...dex.php?title=Advanced_Topics_3C391_-_CASA4.1 3C391 Tutorial Part 2: Image Analysis, Polarization, Self-calibration] which follows on from this one. ...ill carry out the polarization imaging, self-calibration, and polarization analysis and display of the data.
  115 KB (16,402 words) - 19:49, 4 February 2014
• EVLA Continuum Tutorial 3C391-CASA4.1
  ....php?title=EVLA_Advanced_Topics_3C391-CASA4.1 3C391 Tutorial Part 2: Image Analysis, Polarization, Self-calibration] which follows on from this one. ...ill carry out the polarization imaging, self-calibration, and polarization analysis and display of the data.
  115 KB (16,434 words) - 20:08, 6 May 2013
• EVLA Continuum Tutorial 3C391 CASA 4.2
  ...php?title=EVLA_Advanced_Topics_3C391_CASA_4.2 3C391 Tutorial Part 2: Image Analysis, Polarization, Self-calibration] which follows on from this one. ...ill carry out the polarization imaging, self-calibration, and polarization analysis and display of the data.
  116 KB (16,619 words) - 13:26, 6 February 2014
• EVLA Continuum Tutorial 3C391 - CASA 4.2
  ...php?title=EVLA_Advanced_Topics_3C391_CASA_4.2 3C391 Tutorial Part 2: Image Analysis, Polarization, Self-calibration] which follows on from this one. ...ill carry out the polarization imaging, self-calibration, and polarization analysis and display of the data.
  116 KB (16,620 words) - 13:50, 16 December 2014
• EVLA 6cmWideband Tutorial SN2010FZ-CASA3.4
  ...te to identify the frequency/channel of RFI. In particular, we note in our analysis: the same for this final image. Here, we will do some rough analysis on the spectral index to determine
  98 KB (12,933 words) - 17:03, 22 October 2012
• EVLA Continuum Tutorial 3C391-CASA4.3
  ....php?title=EVLA_Advanced_Topics_3C391-CASA4.3 3C391 Tutorial Part 2: Image Analysis, Polarization, Self-calibration] which follows on from this one. ...ill carry out the polarization imaging, self-calibration, and polarization analysis and display of the data.
  120 KB (17,198 words) - 16:25, 20 April 2015
• EVLA Spectral Line Calibration IRC+10216 - workshop
  ...ons. The tutorial continues with continuum subtraction, imaging, and image analysis in
  49 KB (7,632 words) - 21:16, 29 August 2011
• Jupiter: continuum polarization calibration 6.4.1
  ...AO replacement visualization tool for images and cubes is CARTA, the “Cube Analysis and Rendering Tool for Astronomy”. It is available from the '''[https://c ...mage]''' or '''[https://casadocs.readthedocs.io/en/v6.4.1/api/tt/casatasks.analysis.immath.html?highlight=immath immath]''' tasks to do so.
  108 KB (6,833 words) - 14:30, 9 February 2023
• EVLA high frequency Spectral Line tutorial - IRC+10216 part1-CASA3.3
  ...ons. The tutorial continues with continuum subtraction, imaging, and image analysis in
  52 KB (8,201 words) - 12:32, 9 April 2012
• EVLA high frequency Spectral Line tutorial - IRC+10216 part1
  ...ons. The tutorial continues with continuum subtraction, imaging, and image analysis in
  53 KB (8,230 words) - 18:47, 17 May 2012
• EVLA Continuum Tutorial 3C391-CASA4.4
  == Image Analysis and Manipulation == ...e found in [http://casa.nrao.edu/docs/cookbook/casa_cookbook007.html Image Analysis] in the CASA Reference Book.
  163 KB (24,232 words) - 18:34, 16 July 2015
• VLA Continuum Tutorial 3C391-CASA4.6
  == Image Analysis and Manipulation == ...e found in [http://casa.nrao.edu/docs/cookbook/casa_cookbook007.html Image Analysis] in the CASA Reference Book.
  168 KB (25,178 words) - 19:39, 25 August 2016
• EVLA Continuum Tutorial 3C391-CASA4.5
  == Image Analysis and Manipulation == ...e found in [http://casa.nrao.edu/docs/cookbook/casa_cookbook007.html Image Analysis] in the CASA Reference Book.
  163 KB (24,302 words) - 18:13, 10 March 2016
• VLBA Basic Spectral Line Tutorial DRAFT
  ...pectral line projects are in the target imaging and specific spectral line analysis steps.
  52 KB (8,358 words) - 18:00, 14 May 2024
• EVLA 6cmWideband Tutorial SN2010FZ-CASA4.0
  ...te to identify the frequency/channel of RFI. In particular, we note in our analysis: the same for this final image. Here, we will do some rough analysis on the spectral index to determine
  114 KB (15,222 words) - 16:13, 9 November 2012
• EVLA 6cmWideband Tutorial SN2010FZ - CASA4.0
  ...te to identify the frequency/channel of RFI. In particular, we note in our analysis: the same for this final image. Here, we will do some rough analysis on the spectral index to determine
  114 KB (15,237 words) - 20:04, 4 February 2014
• VLA Continuum Tutorial 3C391-CASA4.7
  == Image Analysis and Manipulation == ...e found in [http://casa.nrao.edu/docs/cookbook/casa_cookbook007.html Image Analysis] in the CASA Reference Book.
  170 KB (25,424 words) - 14:50, 6 June 2017
• VLA Continuum Tutorial 3C391-CASA5.0.0
  == Image Analysis and Manipulation == ...und in the [https://casa.nrao.edu/casadocs/casa-5.0.0/image-analysis Image Analysis] section of the CASA documentation.
  178 KB (26,597 words) - 19:03, 30 October 2018
• EVLA 6cmWideband Tutorial SN2010FZ CASA 4.1
  ...te to identify the frequency/channel of RFI. In particular, we note in our analysis: the same for this final image. Here, we will do some rough analysis on the spectral index to determine
  115 KB (15,378 words) - 19:52, 4 February 2014
• EVLA 6cmWideband Tutorial SN2010FZ - CASA 4.1
  ...te to identify the frequency/channel of RFI. In particular, we note in our analysis: the same for this final image. Here, we will do some rough analysis on the spectral index to determine
  115 KB (15,378 words) - 19:51, 4 February 2014
• EVLA 6cmWideband Tutorial SN2010FZ CASA 4.2
  ...te to identify the frequency/channel of RFI. In particular, we note in our analysis: the same for this final image. Here, we will do some rough analysis on the spectral index to determine
  117 KB (15,635 words) - 13:17, 6 February 2014
• EVLA 6cmWideband Tutorial SN2010FZ - CASA 4.2
  ...te to identify the frequency/channel of RFI. In particular, we note in our analysis: the same for this final image. Here, we will do some rough analysis on the spectral index to determine
  117 KB (15,635 words) - 13:53, 16 December 2014
• NGC3256 Band3 Calibration for CASA 4.0
  ...spondingly higher fluxes in all images which will be created later in this analysis. For simplicity, we stay in the following with the 2010 model but will ment
  62 KB (9,285 words) - 07:16, 29 October 2012
• TWHydraBand7 SS12
  ...ve verified that you have the right version of CASA and have access to the analysis utilities module, you can are ready to begin.
  64 KB (10,004 words) - 16:29, 31 May 2012
• MG0414+0534 P-band Spectral Line Tutorial - CASA 5.0.0
  ...and, we only use a small fraction of the total band for data reduction and analysis in this tutorial.
  57 KB (8,166 words) - 15:22, 22 October 2018
• MG0414+0534 P-band Spectral Line Tutorial - CASA 5.4.0
  ...and, we only use a small fraction of the total band for data reduction and analysis in this tutorial.
  53 KB (7,739 words) - 10:46, 25 April 2019
• EVLA 6cmWideband Tutorial SN2010FZ-CASA4.3
  ...te to identify the frequency/channel of RFI. In particular, we note in our analysis: the same for this final image. Here, we will do some rough analysis on the spectral index to determine
  125 KB (15,910 words) - 23:10, 4 June 2015
• VLA CASA Imaging-CASA4.6.0
  ...n the difference is more than half a pixel across the cube. All CASA image analysis tasks are capable of handling such cubes.
  60 KB (9,464 words) - 18:16, 25 May 2016
• VLA CASA Imaging-CASA4.5.2
  ...n the difference is more than half a pixel across the cube. All CASA image analysis tasks are capable of handling such cubes.
  60 KB (9,489 words) - 15:18, 25 May 2016
• MG0414+0534 P-band Spectral Line Tutorial - CASA 5.5.0
  ...and, we only use a small fraction of the total band for data reduction and analysis in this tutorial.
  53 KB (7,864 words) - 12:50, 29 September 2020
• EVLA 6cmWideband Tutorial SN2010FZ-CASA4.4
  ...te to identify the frequency/channel of RFI. In particular, we note in our analysis: the same for this final image. Here, we will do some rough analysis on the spectral index to determine
  127 KB (16,188 words) - 17:52, 13 July 2015
• VLA CASA Imaging-CASA5.4.0
  ...ference in beams is more than half a pixel across the cube. All CASA image analysis tasks are capable of handling such cubes.
  63 KB (9,901 words) - 16:09, 10 June 2019
• VLA CASA Imaging-CASA5.5.0
  ...ference in beams is more than half a pixel across the cube. All CASA image analysis tasks are capable of handling such cubes.
  64 KB (9,998 words) - 12:51, 11 July 2019
• MG0414+0534 P-band Spectral Line Tutorial - CASA 5.7.2
  ...and, we only use a small fraction of the total band for data reduction and analysis in this tutorial.
  57 KB (8,502 words) - 18:49, 22 December 2020
• VLA CASA Imaging-CASA4.7.0
  ...ference in beams is more than half a pixel across the cube. All CASA image analysis tasks are capable of handling such cubes.
  65 KB (10,257 words) - 13:13, 20 April 2017
• VLA CASA Imaging-CASA5.0.0
  ...ference in beams is more than half a pixel across the cube. All CASA image analysis tasks are capable of handling such cubes.
  65 KB (10,334 words) - 15:11, 5 October 2017
• EVLA Wide-Band Wide-Field Imaging: G55.7 3.4-CASA4.0
  ...ing -- so, we will flag the rest of the SPW before continuing with further analysis:
  76 KB (10,592 words) - 15:24, 11 December 2012
• VLA CASA Imaging-CASA6.2.0
  ...izing the task [https://casadocs.readthedocs.io/en/v6.2.0/api/tt/casatasks.analysis.immath.html immath] to manually divide the ''<imagename>.image'' by the ''< ...ference in beams is more than half a pixel across the cube. All CASA image analysis tasks are capable of handling such cubes.
  71 KB (11,202 words) - 16:08, 25 April 2022
• VLA CASA Imaging-CASA5.7.0
  ...ference in beams is more than half a pixel across the cube. All CASA image analysis tasks are capable of handling such cubes.
  66 KB (10,403 words) - 16:09, 7 October 2020
• EVLA Wide-Band Wide-Field Imaging: G55.7 3.4-CASA4.1
  ...ing -- so, we will flag the rest of the SPW before continuing with further analysis:
  77 KB (10,632 words) - 16:09, 2 May 2013
• EVLA Wide-Band Wide-Field Imaging: G55.7 - CASA4.1
  ...ing -- so, we will flag the rest of the SPW before continuing with further analysis:
  77 KB (10,632 words) - 19:57, 4 February 2014
• MG0414+0534 P-band Spectral Line Tutorial - CASA 6.2.0
  ...and, we only use a small fraction of the total band for data reduction and analysis in this tutorial.
  63 KB (9,411 words) - 23:23, 12 February 2023
• EVLA Wide-Band Wide-Field Imaging: G55.7 - CASA4.2
  ...ing -- so, we will flag the rest of the SPW before continuing with further analysis:
  80 KB (11,156 words) - 17:30, 9 May 2014
• VLA CASA Flagging-CASA4.6.0
  ...ill remove amplitude spikes it is, therefore, not recommended for spectral analysis related science such as strong narrow maser lines.
  68 KB (9,089 words) - 18:34, 18 October 2016
• VLA CASA Flagging-CASA4.5.2
  ...ill remove amplitude spikes it is, therefore, not recommended for spectral analysis related science such as strong narrow maser lines.
  68 KB (9,104 words) - 18:34, 18 October 2016
• 3C286 Band6Pol Calibration for CASA 4.5
  ...'' appears in the real part of ''all'' correlations. This complicates the analysis somewhat, but also provides better constraints for estimating and correctin
  76 KB (11,217 words) - 09:38, 10 April 2017
• VLA CASA Flagging-CASA4.7.0
  ...ill remove amplitude spikes it is, therefore, not recommended for spectral analysis related science such as strong narrow maser lines.
  69 KB (9,365 words) - 15:46, 19 July 2017
• 3C286 Band6Pol Calibration for CASA 4.3
  ...'' appears in the real part of ''all'' correlations. This complicates the analysis somewhat, but also provides better constraints for estimating and correctin
  74 KB (10,853 words) - 12:45, 6 October 2021
• VLA CASA Flagging-CASA5.0.0
  ...will remove amplitude spikes, it is therefore not recommended for spectral analysis related science such as strong narrow maser lines.
  73 KB (9,761 words) - 12:19, 1 August 2017
• 3C286 Band6Pol Calibration for CASA 6.5
  ...'' appears in the real part of ''all'' correlations. This complicates the analysis somewhat, but also provides better constraints for estimating and correctin
  75 KB (10,965 words) - 11:02, 21 September 2023
• 3C286 Band6Pol Calibration for CASA 6.5.4
  ...'' appears in the real part of ''all'' correlations. This complicates the analysis somewhat, but also provides better constraints for estimating and correctin
  77 KB (11,049 words) - 14:38, 18 April 2024
• 3C286 Band6Pol Calibration for CASA 6.2
  ...'' appears in the real part of ''all'' correlations. This complicates the analysis somewhat, but also provides better constraints for estimating and correctin
  77 KB (11,223 words) - 16:02, 3 November 2021
• 3C286 Band6Pol Calibration for CASA 5.1
  ...'' appears in the real part of ''all'' correlations. This complicates the analysis somewhat, but also provides better constraints for estimating and correctin
  75 KB (10,912 words) - 14:48, 11 October 2021
• 3C286 Band6Pol Calibration for CASA 5.4
  ...'' appears in the real part of ''all'' correlations. This complicates the analysis somewhat, but also provides better constraints for estimating and correctin
  76 KB (11,034 words) - 16:23, 19 August 2021
• 3C286 Band6Pol Calibration for CASA 5.7
  ...'' appears in the real part of ''all'' correlations. This complicates the analysis somewhat, but also provides better constraints for estimating and correctin
  76 KB (11,030 words) - 16:44, 11 October 2021
• 3C286 Band6Pol Calibration for CASA 6.1
  ...'' appears in the real part of ''all'' correlations. This complicates the analysis somewhat, but also provides better constraints for estimating and correctin
  76 KB (11,036 words) - 09:09, 13 October 2021
• HI 21cm (1.4 GHz) spectral line data reduction: LEDA 44055-CASA6.5.2
  ...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 ...eadthedocs.io/en/v6.5.4/api/tt/casatasks.analysis.imcontsub.html#casatasks.analysis.imcontsub imcontsub] is used post-imaging to subtract the continuum directl
  91 KB (12,686 words) - 20:32, 20 February 2024
• EVLA Wide-Band Wide-Field Imaging: G55.7 3.4-CASA4.3
  ...ing -- so, we will flag the rest of the SPW before continuing with further analysis:
  79 KB (11,069 words) - 23:21, 4 June 2015
• VLA CASA Flagging-CASA5.4.0
  ...smoothing will remove amplitude spikes, it is not recommended for spectral analysis related science (e.g. strong narrow maser lines).</b>
  85 KB (11,750 words) - 19:00, 30 November 2018
• VLA Flagging Intro Tutorial
  ...smoothing will remove amplitude spikes, it is not recommended for spectral analysis related science (e.g. strong narrow maser lines).</b>
  83 KB (11,530 words) - 17:56, 14 May 2024
• VLA CASA Flagging-CASA5.5.0
  ...smoothing will remove amplitude spikes, it is not recommended for spectral analysis related science (e.g. strong narrow maser lines).</b>
  83 KB (11,531 words) - 16:50, 5 July 2019
• VLA CASA Flagging-CASA5.7.0
  ...smoothing will remove amplitude spikes, it is not recommended for spectral analysis related science (e.g. strong narrow maser lines).</b>
  83 KB (11,548 words) - 17:50, 9 November 2020
• VLA CASA Flagging-CASA6.2.0
  ...smoothing will remove amplitude spikes, it is not recommended for spectral analysis related science (e.g. strong narrow maser lines).</b>
  87 KB (12,141 words) - 11:38, 2 May 2022
• VLA CASA Flagging-CASA6.4.1
  ...smoothing will remove amplitude spikes, it is not recommended for spectral analysis related science (e.g. strong narrow maser lines).</b>
  87 KB (12,153 words) - 15:20, 13 February 2023
• VLA CASA Flagging-CASA6.5.4
  ...smoothing will remove amplitude spikes, it is not recommended for spectral analysis related science (e.g. strong narrow maser lines).</b>
  87 KB (12,186 words) - 11:56, 1 March 2024
• AntennaeBand7 Calibration 4.3
  We loop through and using analysis utils, again generating .png files of each calibration. As the bandpass plo
  111 KB (17,150 words) - 09:24, 5 October 2021
• AntennaeBand7 Calibration 4.5
  We loop through and using analysis utils, again generating .png files of each calibration. As the bandpass plo
  112 KB (17,190 words) - 12:29, 11 October 2021
• AntennaeBand7 Calibration 4.4
  We loop through and using analysis utils, again generating .png files of each calibration. As the bandpass plo
  111 KB (17,130 words) - 07:51, 5 October 2021
• AntennaeBand7 Calibration 4.1
  We loop through and using analysis utils, again generating .png files of each calibration. As the bandpass plo
  111 KB (17,131 words) - 10:44, 5 October 2021
• AntennaeBand7 Calibration 4.2
  We loop through and using analysis utils, again generating .png files of each calibration. As the bandpass plo
  111 KB (17,131 words) - 10:06, 5 October 2021
• EVLA Wide-Band Wide-Field Imaging: G55.7 3.4-CASA4.4
  ...ing -- so, we will flag the rest of the SPW before continuing with further analysis:
  83 KB (11,246 words) - 12:30, 3 November 2015
• AntennaeBand7 Calibration 5.1
  We loop through and using analysis utils, again generating .png files of each calibration. '''For what systems
  113 KB (17,396 words) - 16:19, 20 August 2021
• AntennaeBand7 Calibration 5.4
  We loop through and using analysis utils, again generating .png files of each calibration. '''For what systems
  114 KB (17,595 words) - 15:08, 20 August 2021
• AntennaeBand7 Calibration 5.7
  We loop through and using analysis utils, again generating .png files of each calibration. '''For what systems
  114 KB (17,621 words) - 16:05, 19 August 2021
• AntennaeBand7 Calibration 6.4
  We loop through and using analysis utils, again generating .png files of each calibration. '''For what systems
  114 KB (17,545 words) - 13:03, 24 October 2022
• AntennaeBand7 Calibration 6.2
  We loop through and using analysis utils, again generating .png files of each calibration. '''For what systems
  114 KB (17,545 words) - 10:35, 25 August 2022
• AntennaeBand7 Calibration 6.1
  We loop through and using analysis utils, again generating .png files of each calibration. '''For what systems
  114 KB (17,557 words) - 14:43, 20 August 2021
• NGC 5921: red-shifted HI emission 6.5.2
  ...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 ...produced using [https://casadocs.readthedocs.io/en/v6.5.2/api/tt/casatasks.analysis.immoments.html immoments] and displayed with CARTA. Click to enlarge.]]
  94 KB (13,008 words) - 20:51, 31 January 2023
• JVLA - Priori Flagging, Auto-Flagging, and Imaging in CASA-JO
  ...will remove amplitude spikes, it is therefore not recommended for spectral analysis related science, such as HI. Also note that hanning smoothing cannot be rev
  89 KB (12,476 words) - 10:49, 12 April 2016

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