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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
  • ...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) - 13:45, 15 May 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.
    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

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