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  • [[Category:ALMA]][[Category:Imaging]][[Category:Polarization]] ==Full polarization imaging of the target==
    30 KB (4,386 words) - 14:55, 23 October 2023
  • -> adam: linux ALMA cube; juergen: mac os; EVLA polarization IQUV cube -> send also to Adam; skyview fits
    3 KB (407 words) - 14:18, 4 April 2013
  • [[Category:ALMA]][[Category:Imaging]][[Category:Polarization]] ==Full polarization imaging of the target==
    32 KB (4,524 words) - 16:03, 3 April 2018
  • [[Category:ALMA]][[Category:Imaging]][[Category:Polarization]] ==Full polarization imaging of the target==
    31 KB (4,534 words) - 17:29, 11 March 2021
  • [[Category:ALMA]][[Category:Imaging]][[Category:Polarization]] ==Full polarization imaging of the target==
    31 KB (4,537 words) - 17:31, 11 March 2021
  • [[Category:ALMA]][[Category:Imaging]][[Category:Polarization]] ==Full polarization imaging of the target==
    31 KB (4,537 words) - 09:10, 13 October 2021
  • [[Category:ALMA]][[Category:Imaging]][[Category:Polarization]] ==Full polarization imaging of the target==
    31 KB (4,537 words) - 10:20, 1 October 2021
  • cl.addcomponent(flux=1.25, fluxunit='mJy', polarization='Stokes',
    4 KB (618 words) - 02:26, 12 February 2011
  • ...e</tt> turns a model of the sky (2 to 4 dimensions including frequency and polarization) into the visibilities that would be measured with ALMA, (J)VLA, CARMA, SMA ...rrupt - Corrupt the measurement set with thermal noise, phase noise, cross-polarization, etc.
    12 KB (1,773 words) - 13:00, 3 November 2015
  • * Bandpass, polarization leakage and fluxscale calibration was done using an observation of 1934-638 Spectral Windows: (1 unique spectral windows and 1 unique polarization setups)
    29 KB (3,228 words) - 01:23, 1 September 2020
  • ...be used to add phase delay variations, gain fluctuations and drift, cross-polarization, and (coming soon) bandpass and pointing errors to your simulated data. <t ...upt]] - Corrupt the measurement set with thermal noise, phase noise, cross-polarization, etc.
    8 KB (1,321 words) - 14:34, 1 November 2011
  • ...- this is quite rare outside of polarization, and self-calibration of full-polarization projects is not fully validated in any case. 14. In full-polarization datasets, the hif_makeimages page for the polcal has images of polarized in
    25 KB (3,867 words) - 15:19, 13 March 2024
  • ...be used to add phase delay variations, gain fluctuations and drift, cross-polarization, and (coming soon) bandpass and pointing errors to your simulated data. <t ...upt]] - Corrupt the measurement set with thermal noise, phase noise, cross-polarization, etc.
    8 KB (1,275 words) - 18:52, 26 March 2024
  • High Accuracy Spectral Line Polarization Observations ...to 64 independent correlators with different bandwidths, channel numbers, polarization products, and observing frequencies. The final VLA will be able to
    42 KB (6,842 words) - 10:09, 2 July 2012
  • ...391_ctm_mosaic_spw0.ms</tt>. This is what we will use to carry on with our polarization imaging. == Multi-scale Polarization Clean ==
    46 KB (7,311 words) - 14:10, 6 February 2014
  • ...391_ctm_mosaic_spw0.ms</tt>. This is what we will use to carry on with our polarization imaging. == Multi-scale Polarization Clean ==
    46 KB (7,311 words) - 13:51, 16 December 2014
  • ...be used to add phase delay variations, gain fluctuations and drift, cross-polarization, and (coming soon) bandpass and pointing errors to your simulated data. <t ...upt]] - Corrupt the measurement set with thermal noise, phase noise, cross-polarization, etc.
    10 KB (1,479 words) - 13:28, 30 April 2011
  • ...s been tested on dual-polarization ALMA data, and single-, dual-, and full-polarization EVLA data. It supports both the old and new calibration table formats. Plo xcolor: color for XX polarization points (default = blue)
    14 KB (2,237 words) - 13:13, 17 April 2024
  • ...391_ctm_mosaic_spw0.ms</tt>. This is what we will use to carry on with our polarization imaging. == Multi-scale Polarization Clean ==
    47 KB (7,334 words) - 19:42, 4 February 2014
  • ...391_ctm_mosaic_spw0.ms</tt>. This is what we will use to carry on with our polarization imaging. == Multi-scale Polarization Clean ==
    47 KB (7,335 words) - 19:50, 4 February 2014
  • ...391_ctm_mosaic_spw0.ms</tt>. This is what we will use to carry on with our polarization imaging. == Multi-scale Polarization Clean ==
    47 KB (7,549 words) - 16:36, 20 April 2015
  • ...391_ctm_mosaic_spw0.ms</tt>. This is what we will use to carry on with our polarization imaging. == Multi-scale Polarization Clean ==
    47 KB (7,549 words) - 16:32, 20 April 2015
  • ...391_ctm_mosaic_spw0.ms</tt>. This is what we will use to carry on with our polarization imaging. == Multi-scale Polarization Clean ==
    47 KB (7,551 words) - 13:47, 2 June 2015
  • ...391_ctm_mosaic_spw0.ms</tt>. This is what we will use to carry on with our polarization imaging. == Multi-scale Polarization Clean ==
    47 KB (7,436 words) - 16:17, 30 May 2013
  • ...391_ctm_mosaic_spw0.ms</tt>. This is what we will use to carry on with our polarization imaging. == Multi-scale Polarization Clean ==
    47 KB (7,454 words) - 17:12, 22 October 2012
  • * Visibilities are recorded every 2 seconds in full polarization (4 polarization products, (wrongly!) labelled RR,RL,LR,LL). ...than linear. This may seem mostly harmless, but does make a difference for polarization calibration (which we will do later). The following (non-standard) task wil
    46 KB (7,173 words) - 03:27, 8 June 2015
  • ...ystem that it needs to calculate visibilities. If your model doesn't have polarization/Stokes information, we'll add a dummy axis to the image for you. If your i
    6 KB (933 words) - 11:05, 4 November 2012
  • * [[3C286_Polarization]]: Demonstration of the reduction of ALMA continuum polarization toward the quasar 3C286
    6 KB (859 words) - 16:29, 8 January 2018
  • * We ask gaincal to solve for a correction for each "correlation" (i.e., each polarization) by specifying '''gaintype'''="G". ...te tat you see two points in each plot because we have a solution for each polarization.
    20 KB (3,099 words) - 00:21, 7 March 2014
  • ...simulated data: phase delay variations, gain fluctuations and drift, cross-polarization, and (coming soon) bandpass and pointing errors. <tt>sm </tt> also has mor ...sed to corrupt your measurement set with thermal noise, phase noise, cross-polarization, etc., in a more advanced way than is done in <tt>simobserve</tt>. To lear
    12 KB (1,863 words) - 13:00, 3 November 2015
  • [[Category:ALMA]][[Category:Calibration]][[Category:Polarization]] ...ed here is intended to provide an initial example of the reduction of ALMA polarization data. It may be updated in future, and is not necessarily the exact procedu
    76 KB (11,217 words) - 09:38, 10 April 2017
  • [[Category:ALMA]][[Category:Calibration]][[Category:Polarization]] ...ed here is intended to provide an initial example of the reduction of ALMA polarization data. It may be updated in future, and is not necessarily the exact procedu
    74 KB (10,853 words) - 12:45, 6 October 2021
  • [[Category:ALMA]][[Category:Calibration]][[Category:Polarization]] ...ed here is intended to provide an initial example of the reduction of ALMA polarization data. It may be updated in future, and is not necessarily the exact procedu
    77 KB (11,049 words) - 14:38, 18 April 2024
  • [[Category:ALMA]][[Category:Calibration]][[Category:Polarization]] ...ed here is intended to provide an initial example of the reduction of ALMA polarization data. It may be updated in future, and is not necessarily the exact procedu
    75 KB (10,965 words) - 11:02, 21 September 2023
  • [[Category:ALMA]][[Category:Calibration]][[Category:Polarization]] ...ed here is intended to provide an initial example of the reduction of ALMA polarization data. It may be updated in future, and is not necessarily the exact procedu
    77 KB (11,223 words) - 16:02, 3 November 2021
  • [[Category:ALMA]][[Category:Calibration]][[Category:Polarization]] ...ed here is intended to provide an initial example of the reduction of ALMA polarization data. It may be updated in future, and is not necessarily the exact procedu
    76 KB (11,034 words) - 16:23, 19 August 2021
  • [[Category:ALMA]][[Category:Calibration]][[Category:Polarization]] ...ed here is intended to provide an initial example of the reduction of ALMA polarization data. It may be updated in future, and is not necessarily the exact procedu
    76 KB (11,030 words) - 16:44, 11 October 2021
  • [[Category:ALMA]][[Category:Calibration]][[Category:Polarization]] ...ed here is intended to provide an initial example of the reduction of ALMA polarization data. It may be updated in future, and is not necessarily the exact procedu
    75 KB (10,912 words) - 14:48, 11 October 2021
  • [[Category:ALMA]][[Category:Calibration]][[Category:Polarization]] ...ed here is intended to provide an initial example of the reduction of ALMA polarization data. It may be updated in future, and is not necessarily the exact procedu
    76 KB (11,036 words) - 09:09, 13 October 2021
  • ...simulated data: phase delay variations, gain fluctuations and drift, cross-polarization, and bandpass and pointing errors. '[https://casa.nrao.edu/docs/CasaRef/Ca
    7 KB (1,016 words) - 12:22, 21 March 2024
  • ...simulated data: phase delay variations, gain fluctuations and drift, cross-polarization, and bandpass and pointing errors. {{simulator_6.5.4}} also has more flexi
    6 KB (922 words) - 18:37, 26 March 2024
  • ...simulated data: phase delay variations, gain fluctuations and drift, cross-polarization, and bandpass and pointing errors. '[https://casa.nrao.edu/docs/CasaRef/Ca
    7 KB (1,115 words) - 16:25, 12 February 2024
  • Spectral Windows: (16 unique spectral windows and 1 unique polarization setups) * Visibilities are recorded every 2 seconds in full polarization (4 polarization products, (wrongly!) labelled RR,RL,LR,LL).
    52 KB (7,963 words) - 17:54, 3 January 2017
  • Spectral Windows: (16 unique spectral windows and 1 unique polarization setups) * Visibilities are recorded every 2 seconds in full polarization (4 polarization products, (wrongly!) labelled RR,RL,LR,LL).
    53 KB (8,002 words) - 17:53, 3 January 2017
  • Spectral Windows: (16 unique spectral windows and 1 unique polarization setups) * Visibilities are recorded every 2 seconds in full polarization (4 polarization products, (wrongly!) labelled RR,RL,LR,LL).
    52 KB (7,963 words) - 16:06, 10 October 2016
  • Spectral Windows: (16 unique spectral windows and 1 unique polarization setups) * Visibilities are recorded every 2 seconds in full polarization (4 polarization products, (wrongly!) labelled RR,RL,LR,LL).
    52 KB (7,964 words) - 17:49, 3 January 2017
  • ...simulated data: phase delay variations, gain fluctuations and drift, cross-polarization, and (coming soon) bandpass and pointing errors. <tt>sm </tt> also has mor ...sed to corrupt your measurement set with thermal noise, phase noise, cross-polarization, etc., in a more advanced way than is done in <tt>simobserve</tt>. To lear
    14 KB (2,193 words) - 10:17, 20 November 2015

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