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- == Observational approaches to enable successful polarization calibration == == Instrumental polarization: technical aspects ==481 bytes (48 words) - 16:32, 30 July 2010
- [[Category:ALMA]][[Category:Polarization]][[Category:Continuum]] These SV observations have been taken with the aim of testing ALMA polarization capabilities at Band 6 (233 GHz, 1 mm).7 KB (1,126 words) - 13:33, 18 October 2023
- [[Category:ALMA]][[Category:Calibration]][[Category:Continuum]][[Category:Polarization]]513 bytes (65 words) - 11:09, 4 August 2014
- [[Category:ALMA]][[Category:Imaging]][[Category:Continuum]][[Category:Polarization]]509 bytes (65 words) - 11:09, 4 August 2014
- Spectral Windows: (2 unique spectral windows and 1 unique polarization setups) ...larization leakage on 0137+331. In this step we solve for the instrumental polarization. We will assume here our calibrator has unknown polarisation (poltype='D+QU25 KB (3,544 words) - 13:00, 13 February 2023
- 63 bytes (5 words) - 13:01, 13 February 2023
- ...indows with 64 channels each. The observation was set up to allow for full polarization calibration. The first step of polarization calibration is to first obtain a decent Stokes I (RR and LL) calibration. T123 KB (17,782 words) - 13:42, 22 April 2024
- #REDIRECT [[VLA Polarization pipe Tutorial]]44 bytes (5 words) - 15:19, 22 May 2023
- Spectral Windows: (14 unique spectral windows and 1 unique polarization setups) * 0137+331 (polarization leakage calibrator)108 KB (6,833 words) - 14:30, 9 February 2023
- * 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
- #REDIRECT [[ATCA Continuum Polarization Tutorial NGC612-CASA4.7]]65 bytes (7 words) - 18:32, 12 October 2016
- Spectral Windows: (1 unique spectral windows and 1 unique polarization setups) ...ng solution interval to do the bandpass solution. Because we're processing polarization data from an Az/El telescope we switch on parallactic angle rotation using33 KB (5,218 words) - 18:24, 6 June 2022
- #REDIRECT [[CASA Guides:ATCA Advanced Continuum Polarization Tutorial NGC612-CASA4.7]]86 bytes (10 words) - 22:54, 28 July 2016
- 125 bytes (16 words) - 18:32, 8 February 2024
- ...r and memory. This CASA guide was also used as basis for a presentation on polarization calibration at the 7th VLA data reduction workshop: [https://science.nrao.e ...steps and final imaging can be performed: ['https://casa.nrao.edu/Data/VLA/Polarization/TDRW0001_calibrated_CASA6.5.4.ms.tgz '] (size: 11 GB). It is recommended to145 KB (20,668 words) - 18:14, 8 February 2024
- ...indows with 64 channels each. The observation was set up to allow for full polarization calibration. ...alibrated measurement set, we have created a starting dataset on which the polarization calibration steps and final imaging can be performed: [https://casa.nrao.ed131 KB (17,960 words) - 19:34, 20 November 2019
- #REDIRECT [[Polarization Calibration based on CASA pipeline standard reduction: The radio galaxy 3C7113 bytes (14 words) - 18:43, 19 September 2019
- #REDIRECT [[CASA Guides:Polarization Calibration based on CASA pipeline standard reduction: The radio galaxy 3C7125 bytes (16 words) - 12:34, 3 April 2020
- ...r and memory. This CASA guide was also used as basis for a presentation on polarization calibration at the 7th VLA data reduction workshop: [https://science.nrao.e ...alibrated measurement set, we have created a starting dataset on which the polarization calibration steps and final imaging can be performed: [ftp://ftp.aoc.nrao.e131 KB (17,967 words) - 18:25, 1 April 2021
- ...r and memory. This CASA guide was also used as basis for a presentation on polarization calibration at the 7th VLA data reduction workshop: [https://science.nrao.e ...alibrated measurement set, we have created a starting dataset on which the polarization calibration steps and final imaging can be performed: [''ftp://ftp.aoc.nrao131 KB (18,080 words) - 15:45, 23 October 2020
- ...r and memory. This CASA guide was also used as basis for a presentation on polarization calibration at the 7th VLA data reduction workshop: [https://science.nrao.e ...steps and final imaging can be performed: ['https://casa.nrao.edu/Data/VLA/Polarization/TDRW0001_calibrated_CASA6.2.1.ms.tgz '] (size: 10 GB). It is recommended to147 KB (20,282 words) - 17:44, 6 December 2022
- ...r and memory. This CASA guide was also used as basis for a presentation on polarization calibration at the 7th VLA data reduction workshop: [https://science.nrao.e ...steps and final imaging can be performed: ['https://casa.nrao.edu/Data/VLA/Polarization/TDRW0001_calibrated_CASA6.4.1.ms.tgz '] (size: 11 GB). It is recommended to149 KB (20,704 words) - 12:28, 9 January 2024
- #REDIRECT [[CASA Guides:Polarization Calibration based on CASA pipeline standard reduction: The radio galaxy 3C7148 bytes (17 words) - 18:10, 1 April 2021
- #REDIRECT [[CASA Guides:Polarization Calibration based on CASA pipeline standard reduction: The radio galaxy 3C7125 bytes (16 words) - 18:42, 19 September 2019
- ...r and memory. This CASA guide was also used as basis for a presentation on polarization calibration at the 7th VLA data reduction workshop: [https://science.nrao.e ...alibrated measurement set, we have created a starting dataset on which the polarization calibration steps and final imaging can be performed: ['https://casa.nrao.e136 KB (18,625 words) - 12:00, 16 December 2021
Page text matches
- == Observational approaches to enable successful polarization calibration == == Instrumental polarization: technical aspects ==481 bytes (48 words) - 16:32, 30 July 2010
File:3C391 full pol image.png ...nd red vectors show the orientation of the magnetic field where the linear polarization is >5 sigma.(608 × 799 (121 KB)) - 17:12, 18 May 2010- * [[CASA Guides:New Polarization casa guide casa 5.4.0]] * [[CASA Guides:New Polarization casa guide casa 6.1.2.7-pipeline-2020.1.0.36]]429 bytes (51 words) - 19:49, 19 December 2022
File:Plotcal-3C286-G0-bandpass-R.png bandpass solutions for 3C 286, R polarization(658 × 580 (45 KB)) - 10:18, 6 May 2010File:Plotcal-3C286-G0-bandpass-L.png bandpass solutions for 3C 286, L polarization(658 × 580 (45 KB)) - 10:19, 6 May 2010- #REDIRECT [[VLA Polarization pipe Tutorial]]44 bytes (5 words) - 15:19, 22 May 2023
File:Plotms-3C286-RRbandpass.png Illustration of bandpass, RR polarization, 3C 286(808 × 629 (73 KB)) - 17:57, 24 May 2010File:Plotcal-3C286-G0-phase-L.png Phase solutions for 3C 286, L polarization, from plotcal(812 × 612 (61 KB)) - 16:51, 9 June 2010File:Plotcal-3C286-G0all-phase-R-ea05.png initial phase calibration, R polarization, ea05(858 × 655 (21 KB)) - 15:19, 6 July 2015File:Plotcal-J1822-0398-phase-R.png gain phase solutions for J1822-0398, R polarization(812 × 612 (94 KB)) - 18:39, 9 June 2010File:Plotcal-J1822-0398-phase-L.png gain phase solutions for J1822-0398, L polarization(812 × 612 (91 KB)) - 18:42, 9 June 2010File:Figure21.png Phase solutions for the X polarization for each scan of the first dataset.(1,218 × 702 (91 KB)) - 11:30, 23 May 2012- #REDIRECT [[ATCA Continuum Polarization Tutorial NGC612-CASA4.7]]65 bytes (7 words) - 18:32, 12 October 2016
File:Figure20a.png Phase solutions for the X polarization for every integration time of the first dataset.(1,141 × 625 (112 KB)) - 11:29, 23 May 2012File:ComparisonI 6.5.4.png Total intensity image of the polarization calibrator.(1,141 × 575 (244 KB)) - 16:43, 10 October 2023File:Pband delaycal.png Fig.4. Delays for each antenna and each polarization. Plot made with ‘plotcal’(812 × 612 (20 KB)) - 15:47, 18 August 2017- #REDIRECT [[CASA Guides:ATCA Advanced Continuum Polarization Tutorial NGC612-CASA4.7]]86 bytes (10 words) - 22:54, 28 July 2016
File:3C391 full pol image vector settings.png Data Display Options GUI for the position angle vectors in the final polarization image of 3C391.(493 × 694 (45 KB)) - 17:16, 18 May 2010- #REDIRECT [[Polarization Calibration based on CASA pipeline standard reduction: The radio galaxy 3C7113 bytes (14 words) - 18:43, 19 September 2019
- * [[ATCA_Continuum_Polarization_Tutorial_NGC612-CASA4.7| ATCA Continuum Polarization Tutorial]] (CASA 4.7 version) ...ed_Continuum_Polarization_Tutorial_NGC612-CASA4.7| ATCA Advanced Continuum Polarization Tutorial]] (CASA 4.7 version)598 bytes (84 words) - 18:52, 2 September 2020
File:Vlba casacal ChoosingRefant1.png ...ce Antenna, 4C39.25 phase vs frequency, BR-LA baseline, left-hand circular polarization(1,026 × 625 (93 KB)) - 17:06, 27 June 2022File:Vlba casacal ChoosingRefant2.png ...ce Antenna, 4C39.25 amplitude vs freq, OV-PT baseline, right-hand circular polarization(1,025 × 630 (99 KB)) - 17:07, 27 June 2022File:Vlba casacal ChoosingRefant1 RR.png ...tenna, Phase vs Frequency for 4C39.25, BR-LA baseline, right-hand circular polarization.(1,026 × 627 (92 KB)) - 17:06, 27 June 2022- #REDIRECT [[CASA Guides:Polarization Calibration based on CASA pipeline standard reduction: The radio galaxy 3C7125 bytes (16 words) - 18:42, 19 September 2019
- #REDIRECT [[CASA Guides:Polarization Calibration based on CASA pipeline standard reduction: The radio galaxy 3C7125 bytes (16 words) - 12:34, 3 April 2020
File:Vlba casacal ChoosingRefant2 LL.png ...na, Amplitude vs frequency for 4C39.25, OV-PT baseline, left-hand circular polarization.(1,025 × 627 (93 KB)) - 17:07, 27 June 2022- [[Category:ALMA]][[Category:Calibration]][[Category:Continuum]][[Category:Polarization]]513 bytes (65 words) - 11:09, 4 August 2014
- [[Category:ALMA]][[Category:Imaging]][[Category:Continuum]][[Category:Polarization]]509 bytes (65 words) - 11:09, 4 August 2014
- #REDIRECT [[CASA Guides:Polarization Calibration based on CASA pipeline standard reduction: The radio galaxy 3C7148 bytes (17 words) - 18:10, 1 April 2021
File:ComparisonU 6.5.4.png U image of the polarization calibrator. Image on left has D-term correction applied. The right image(1,141 × 575 (366 KB)) - 16:46, 10 October 2023File:ComparisonQ 6.5.4.png Q image of polarization calibrator. The left image is with D-term calibration. The right image is(1,141 × 575 (392 KB)) - 16:45, 10 October 2023File:Pband flagchan.png Fig.2. Flagging of calibrator 3C48. Shown are the XX and YY polarization on antenna ea01, both before and after flagging the bad channels. The color(1,880 × 697 (497 KB)) - 16:33, 18 August 2017- ...based_on_CASA_pipeline_standard_reduction:_The_radio_galaxy_3C75-CASA6.5.4 Polarization Calibration based on CASA pipeline standard reduction: The radio galaxy 3C7 ...based_on_CASA_pipeline_standard_reduction:_The_radio_galaxy_3C75-CASA6.4.1 Polarization Calibration based on CASA pipeline standard reduction: The radio galaxy 3C721 KB (2,724 words) - 12:03, 1 March 2024
- ** [[Jupiter: continuum polarization calibration]]585 bytes (71 words) - 19:16, 18 September 2018
- [[Category:ALMA]][[Category:Polarization]][[Category:Continuum]] These SV observations have been taken with the aim of testing ALMA polarization capabilities at Band 6 (233 GHz, 1 mm).7 KB (1,126 words) - 13:33, 18 October 2023
- cl.addcomponent(flux=1.25, fluxunit='mJy', polarization='Stokes',991 bytes (162 words) - 15:12, 29 February 2012
- == Leakage a.k.a. Cross-polarization == * random Gaussian (time-independent) complex cross-polarization leakage terms, with specified real and imaginary amplitudes, and an optiona9 KB (1,379 words) - 17:17, 7 November 2012
- == Leakage a.k.a. Cross-polarization == * random Gaussian (time-independent) complex cross-polarization leakage terms, with specified real and imaginary amplitudes, and an optiona9 KB (1,379 words) - 15:36, 23 January 2018
- ...ples for common general-use cases such as spectral line, continuum, linear polarization, and mosaicking. However, the results demonstrated here are specific to th === Polarization Calibration based on CASA pipeline standard reduction: The radio galaxy 3C713 KB (1,866 words) - 17:24, 25 March 2024
- ...s to pre-apply before solving for a particular effect (gain or bandpass or polarization). The user (''not'' the task!) specifies a calibration table to store the s * {{polcal}}: polarization calibration;6 KB (862 words) - 17:03, 27 March 2013
- ...tion, Imaging]] and [[EVLA Advanced Topics 3C391-CASA3.4 | Image Analysis, Polarization, Self-calibration]] ...ion, Imaging]] and [[ EVLA Advanced Topics 3C391-CASA3.3 | Image Analysis, Polarization, Self-calibration ]]8 KB (970 words) - 16:45, 10 June 2013
- [[Category:ALMA]][[Category:Imaging]][[Category:Polarization]] ==Full polarization imaging of the target==28 KB (4,145 words) - 09:41, 14 September 2017
- [[Category:ALMA]][[Category:Imaging]][[Category:Polarization]] ==Full polarization imaging of the target==28 KB (4,149 words) - 09:48, 10 April 2017
- == Polarization Imaging == ...tains an "animator" or pane with movie controls. One can step through the polarization axis, displaying the images for the different polarizations.29 KB (4,851 words) - 12:30, 9 April 2012
- ...bserve turns a model of the sky (2 to 4 dimensions including frequency and polarization) into the visibilities that would be measured with ALMA, (E)VLA, CARMA, SMA ...upt]] - Corrupt the measurement set with thermal noise, phase noise, cross-polarization, etc.8 KB (1,207 words) - 13:02, 3 November 2015
- [[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
- ...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
- ...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 wil46 KB (7,173 words) - 03:27, 8 June 2015
- Spectral Windows: (1 unique spectral windows and 1 unique polarization setups) ...ng solution interval to do the bandpass solution. Because we're processing polarization data from an Az/El telescope we switch on parallactic angle rotation using33 KB (5,218 words) - 18:24, 6 June 2022
- ...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 i6 KB (933 words) - 11:05, 4 November 2012
- * [[3C286_Polarization]]: Demonstration of the reduction of ALMA continuum polarization toward the quasar 3C2866 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 lear12 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 procedu76 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 procedu74 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 procedu77 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 procedu75 KB (10,965 words) - 11:02, 21 September 2023
- 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 (7,927 words) - 23:29, 11 March 2016
- [[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 procedu77 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 procedu76 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 procedu76 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 procedu75 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 procedu76 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/Ca7 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 flexi6 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/Ca7 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 lear14 KB (2,193 words) - 10:17, 20 November 2015
- ...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 lear14 KB (2,192 words) - 12:59, 3 November 2015
- Spectral Windows: (19 unique spectral windows and 1 unique polarization setups) * Visibilities are recorded every 2 seconds in full polarization (4 polarization products labelled XX,XY,YX,YY).48 KB (7,722 words) - 12:39, 5 November 2020