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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 fits3 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 in25 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 to42 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