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  • == 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 2010
  • File: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 2010
  • File:Plotcal-3C286-G0-phase-L.png
    Phase solutions for 3C 286, L polarization, from plotcal
    (812 × 612 (61 KB)) - 16:51, 9 June 2010
  • File:Plotcal-3C286-G0all-phase-R-ea05.png
    initial phase calibration, R polarization, ea05
    (858 × 655 (21 KB)) - 15:19, 6 July 2015
  • File:Plotcal-J1822-0398-phase-R.png
    gain phase solutions for J1822-0398, R polarization
    (812 × 612 (94 KB)) - 18:39, 9 June 2010
  • File:Plotcal-J1822-0398-phase-L.png
    gain phase solutions for J1822-0398, L polarization
    (812 × 612 (91 KB)) - 18:42, 9 June 2010
  • File: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 2012
  • File:ComparisonI 6.5.4.png
    Total intensity image of the polarization calibrator.
    (1,141 × 575 (244 KB)) - 16:43, 10 October 2023
  • File: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 3C7
    113 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 2022
  • File: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 2022
  • File: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 3C7
    125 bytes (16 words) - 18:42, 19 September 2019
  • #REDIRECT [[CASA Guides:Polarization Calibration based on CASA pipeline standard reduction: The radio galaxy 3C7
    125 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 3C7
    148 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 2023
  • File: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 2023
  • File: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 3C7
    21 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 optiona
    9 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 optiona
    9 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 3C7
    13 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 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
  • 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 using
    33 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 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
  • 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 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
  • ...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 (2,192 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
  • 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).
    49 KB (7,720 words) - 14:49, 16 January 2019
  • 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).
    53 KB (8,386 words) - 15:14, 19 July 2017
  • ANTENNA POLARIZATION table.f10 table.f17_TSM1 table.f21 table.f26 tab
    8 KB (1,344 words) - 15:06, 9 August 2012
  • 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).
    53 KB (8,399 words) - 13:11, 20 April 2017
  • 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).
    49 KB (7,876 words) - 05:09, 10 November 2020
  • ...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 (2,261 words) - 09:02, 14 December 2018
  • 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).
    55 KB (8,694 words) - 19:20, 29 August 2017
  • 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).
    55 KB (8,718 words) - 17:33, 13 February 2018
  • 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).
    55 KB (8,756 words) - 12:10, 11 July 2018
  • 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).
    56 KB (8,698 words) - 11:34, 2 May 2022
  • Gaintype: ‘gaintype’=‘G’ will cause gaincal to derive solutions for each polarization independently. This becomes more important if you have a polarized source or a source whose polarization state you do not know. If your source
    22 KB (3,254 words) - 12:48, 27 September 2023
  • ...nd a STOKES axis. This is true even if the data and simulation are single-polarization continuum data, in which case the FREQUENCY and STOKES axes can be "singlet # first index indexes polarization (there are two --XX, YY); second is null (probably SPW or IF, nominally)-
    12 KB (2,073 words) - 10:46, 15 March 2022
  • * [[3C286_Polarization]]: Demonstration of the reduction of ALMA continuum polarization toward the quasar 3C286
    8 KB (1,075 words) - 21:06, 14 December 2017
  • ...w the behavior of the calibration tables as a function of time, frequency, polarization, etc., and analytical numbers describe the amount of flagging, derived flux ...imilar to an ''abs(sin)'' or a 'bouncing' signal across a baseband for one polarization or, in other terms, various numbers of 'V' shapes in the data, usually in t
    32 KB (5,038 words) - 17:10, 12 September 2023
  • 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).
    54 KB (8,446 words) - 19:06, 29 February 2024
  • ...simulated data: phase delay variations, gain fluctuations and drift, cross-polarization, and bandpass and pointing errors. '[https://casa.nrao.edu/docs/CasaRef/Ca
    8 KB (1,252 words) - 17:23, 15 February 2023
  • * [[3C286_Polarization]]: Demonstration of the reduction of ALMA continuum polarization toward the quasar 3C286. Validated for CASA 6.5.4.
    8 KB (1,173 words) - 12:33, 22 April 2024
  • Gaintype: ‘gaintype’=‘G’ will cause gaincal to derive solutions for each polarization independently. This becomes more important if you have a polarized source or a source whose polarization state you do not know. If your source
    23 KB (3,449 words) - 17:16, 13 October 2023
  • ...d, we see no obvious bad data. Note that the low points are actually cross-polarization data; you can see this by entering: Which will display only the RR, LL data and not the cross-polarization data (LR, RL).
    34 KB (5,086 words) - 17:13, 3 February 2023
  • ...set to 1e-08. Anything less than this is unlikely to be real. Since for polarization observations we do not wish to keep the cross-hand visibilities if the para
    7 KB (1,170 words) - 16:58, 8 May 2016
  • 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+QU
    25 KB (3,544 words) - 13:00, 13 February 2023
  • ...=EVLA_Advanced_Topics_3C391-CASA3.3 3C391 Tutorial Part 2: Image Analysis, Polarization, Self-calibration] ...ed spectral windows, centered at 4.6 and 7.5 GHz, and were set up for full polarization calibration.
    94 KB (13,931 words) - 12:32, 9 April 2012
  • ...annels and their widths in frequency and velocity units. For each spw, the polarization products and the receiver bands are also listed. ...The 37-39GHz range of ea18 varies considerably more. In fact this antenna, polarization and baseband shows a deformatter timing error (more in the following stage
    50 KB (7,973 words) - 18:32, 2 February 2018
  • ...annels and their widths in frequency and velocity units. For each spw, the polarization products and the receiver bands are also listed. ...The 37-39GHz range of ea18 varies considerably more. In fact this antenna, polarization and baseband shows a deformatter timing error (more in the following stage
    52 KB (8,196 words) - 14:51, 13 February 2018
  • Spectral Windows: (18 unique spectral windows and 1 unique polarization setups)
    11 KB (1,530 words) - 21:09, 1 March 2012
  • ...libration_based_on_CASA_pipeline_standard_reduction:_The_radio_galaxy_3C75 Polarization Calibration based on CASA pipeline (3C75)]. ...annels and their widths in frequency and velocity units. For each spw, the polarization products and the receiver bands are also listed. The real id is the spw id
    60 KB (9,393 words) - 19:00, 28 February 2022
  • ...calibration. 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 The first step of polarization calibration is to first obtain a decent Stokes I (RR and LL) calibration. T
    121 KB (17,444 words) - 18:01, 24 May 2023
  • ...libration_based_on_CASA_pipeline_standard_reduction:_The_radio_galaxy_3C75 Polarization Calibration based on CASA pipeline (3C75)]. ...annels and their widths in frequency and velocity units. For each spw, the polarization products and the receiver bands are also listed. The real id is the spw id
    62 KB (9,694 words) - 13:46, 17 January 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. T
    123 KB (17,782 words) - 13:42, 22 April 2024
  • Spectral Windows: (18 unique spectral windows and 1 unique polarization setups)
    11 KB (1,581 words) - 13:47, 1 May 2013
  • ...annels and their widths in frequency and velocity units. For each spw, the polarization products and the receiver bands are also listed. The real id is the spw id ...when they have otherwise the exact same properties (i.e. same spw, field, polarization, etc.). When data are flagged, the connector will not be plotted, so only c
    59 KB (9,223 words) - 19:22, 18 June 2019
  • ...35 INFO listobs Spectral Windows: (1 unique spectral windows and 1 unique polarization setups) ...window is sampled with 256 channels each 7.8 kHz wide. There are no cross-polarization data (note that 'Corrs' is set to only 'RR LL').
    51 KB (6,414 words) - 17:21, 4 May 2010
  • ...simulated data: phase delay variations, gain fluctuations and drift, cross-polarization, and bandpass and pointing errors. '[https://casa.nrao.edu/docs/CasaRef/Ca
    10 KB (1,558 words) - 15:55, 21 March 2024
  • Spectral Windows: (8 unique spectral windows and 1 unique polarization setups)
    9 KB (1,096 words) - 16:50, 12 April 2024
  • 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
  • ...ing personality, using dual polarization with one spectral windows in each polarization. The spectral window has a bandwidth of 32 MHz divided into 256 spectral c
    21 KB (3,417 words) - 16:56, 30 April 2024
  • ...d, we see no obvious bad data. Note that the low points are actually cross-polarization data; if you want to only look at the right and left polarizations, enter ...w-amplitude points in your data are probably not junk. They are real cross-polarization data. Flagging those data will cause grief later on. Take a look at the tut
    31 KB (4,564 words) - 02:04, 2 June 2015
  • ...libration_based_on_CASA_pipeline_standard_reduction:_The_radio_galaxy_3C75 Polarization Calibration based on CASA pipeline (3C75)]. ...uency and velocity units. The list also includes correlator setups such as polarization products, bits, frequency band and band type, and the baseband. The 'Median
    69 KB (10,685 words) - 12:46, 22 December 2023
  • ...hp?title=EVLA_Advanced_Topics_3C391 3C391 Tutorial Part 2: Image Analysis, Polarization, Self-calibration] which follows on from this one. ...ed spectral windows, centered at 4.6 and 7.5 GHz, and were set up for full polarization calibration.
    117 KB (17,075 words) - 16:16, 30 May 2013
  • ...=EVLA_Advanced_Topics_3C391-CASA3.4 3C391 Tutorial Part 2: Image Analysis, Polarization, Self-calibration] which follows on from this one. ...ed spectral windows, centered at 4.6 and 7.5 GHz, and were set up for full polarization calibration.
    116 KB (17,150 words) - 17:11, 22 October 2012
  • Spectral Windows: (1 unique spectral windows and 1 unique polarization setups) 3) Calculate the weights based on the rms of the cross-polarization products (currently not supported in [https://casadocs.readthedocs.io/en/v6
    28 KB (3,634 words) - 19:56, 5 October 2021
  • ...d, we see no obvious bad data. Note that the low points are actually cross-polarization data; you can see this by entering: ...w-amplitude points in your data are probably not junk. They are real cross-polarization data. Flagging those data will cause grief later on. Take a look at the tut
    29 KB (4,241 words) - 17:16, 2 February 2023
  • ...annels and their widths in frequency and velocity units. For each spw, the polarization products and the receiver bands are also listed. The real id is the spw id ...when they have otherwise the exact same properties (i.e. same spw, field, polarization, etc.). When data are flagged, the connector will not be plotted, so only c
    60 KB (9,524 words) - 17:19, 26 November 2019
  • ...between "G" and "T" (the former generates solutions independently for each polarization, and the latter averages two polarizations before determining the solutions
    12 KB (1,779 words) - 11:15, 5 March 2018
  • ...in order to measure the multi-band delay (MBD). The target dataset is dual polarization (important since the source is circularly polarized) and frequencies that a FRING1: Time= 0/ 07 36 19, Polarization = 1
    45 KB (7,155 words) - 16:38, 13 May 2022
  • leakage -- add cross polarization corruption of this fractional magnitude
    12 KB (1,706 words) - 11:53, 1 December 2010
  • Spectral Windows: (1 unique spectral windows and 1 unique polarization setups) 3) Calculate the weights based on the rms of the cross-polarization products (currently not supported in [https://casadocs.readthedocs.io/en/v6
    30 KB (3,840 words) - 17:11, 22 February 2024
  • Spectral Windows: (1 unique spectral windows and 1 unique polarization setups) 3) Calculate the weights based on the rms of the cross-polarization products (currently not supported in [https://casadocs.readthedocs.io/en/v6
    30 KB (3,847 words) - 16:55, 22 February 2024
  • ...annels and their widths in frequency and velocity units. For each spw, the polarization products and the receiver bands are also listed. The real id is the spw id ...when they have otherwise the exact same properties (i.e. same spw, field, polarization, etc.). When data are flagged, the connector will not be plotted, so only c
    60 KB (9,408 words) - 18:19, 7 July 2021
  • ...=EVLA_Advanced_Topics_3C391-CASA4.1 3C391 Tutorial Part 2: Image Analysis, Polarization, Self-calibration] which follows on from this one. ...ed spectral windows, centered at 4.6 and 7.5 GHz, and were set up for full polarization calibration.
    115 KB (16,434 words) - 20:08, 6 May 2013
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) Spectral Windows: (6 unique spectral windows and 1 unique polarization setups)
    33 KB (5,060 words) - 17:27, 29 April 2024
  • * the pipeline assumes that polarization information is not required; # G = calibrator useful to determine Polarization Angle
    19 KB (2,740 words) - 16:02, 20 June 2010
  • ...peline to the specifics of their observations including spectral line, and polarization. In the following we will also explain how to adapt the pipeline, e.g., for • No polarization calibration (yet) but can use pipeline output as starting data for
    83 KB (12,631 words) - 16:13, 10 October 2016
  • ...peline to the specifics of their observations including spectral line, and polarization. In the following we will also explain how to adapt the pipeline, e.g., for • No polarization calibration (yet) but can use pipeline output as starting data for
    84 KB (12,632 words) - 17:59, 29 March 2017
  • ...annels and their widths in frequency and velocity units. For each spw, the polarization products and the receiver bands are also listed. The real id is the spw id ...when they have otherwise the exact same properties (i.e. same spw, field, polarization, etc.). When data are flagged, the connector will not be plotted, so only c
    62 KB (9,729 words) - 17:59, 1 October 2021
  • ...tle=Advanced_Topics_3C391_-_CASA4.1 3C391 Tutorial Part 2: Image Analysis, Polarization, Self-calibration] which follows on from this one. ...ed spectral windows, centered at 4.6 and 7.5 GHz, and were set up for full polarization calibration.
    115 KB (16,402 words) - 19:49, 4 February 2014
  • ...=EVLA_Advanced_Topics_3C391-CASA4.3 3C391 Tutorial Part 2: Image Analysis, Polarization, Self-calibration] which follows on from this one. ...ed spectral windows, centered at 4.6 and 7.5 GHz, and were set up for full polarization calibration.
    120 KB (17,198 words) - 16:25, 20 April 2015
  • ...hannels and their widths in frequency and velocity units. For each spw the polarization products and the receiver bands are listed, too. ...The 37-39GHz range of ea18 varies considerably more. In fact this antenna, polarization and baseband shows a deformatter timing error (more in the following stage
    85 KB (13,006 words) - 18:57, 19 May 2017
  • ...EVLA_Advanced_Topics_3C391_CASA_4.2 3C391 Tutorial Part 2: Image Analysis, Polarization, Self-calibration] which follows on from this one. ...ed spectral windows, centered at 4.6 and 7.5 GHz, and were set up for full polarization calibration.
    116 KB (16,619 words) - 13:26, 6 February 2014
  • ...EVLA_Advanced_Topics_3C391_CASA_4.2 3C391 Tutorial Part 2: Image Analysis, Polarization, Self-calibration] which follows on from this one. ...ed spectral windows, centered at 4.6 and 7.5 GHz, and were set up for full polarization calibration.
    116 KB (16,620 words) - 13:50, 16 December 2014
  • polarization in the total (subband) bandwidth. Depending on the array average of the offsets determined for each polarization.
    25 KB (3,850 words) - 19:58, 17 August 2011
  • ...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.ed
    131 KB (17,960 words) - 19:34, 20 November 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: [ftp://ftp.aoc.nrao.e
    131 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.nrao
    131 KB (18,080 words) - 15:45, 23 October 2020
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) ...above plot and the corresponding plots for the other spectral windows and polarization products. The purpose here is to get the phases approximately flat as a fu
    61 KB (9,010 words) - 10:28, 18 April 2013
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) ...above plot and the corresponding plots for the other spectral windows and polarization products. The purpose here is to get the phases approximately flat as a fu
    61 KB (9,025 words) - 11:19, 29 November 2013
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) ...above plot and the corresponding plots for the other spectral windows and polarization products. The purpose here is to get the phases approximately flat as a fu
    62 KB (9,285 words) - 07:16, 29 October 2012
  • Spectral Windows: (14 unique spectral windows and 1 unique polarization setups) 3) Calculate the weights based on the rms of the cross-polarization products (currently not supported in {{statwt}}).
    42 KB (5,500 words) - 13:13, 4 October 2017
  • ...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.e
    136 KB (18,625 words) - 12:00, 16 December 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 ...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 to
    145 KB (20,668 words) - 18:14, 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_CASA6.4.1.ms.tgz '] (size: 11 GB). It is recommended to
    149 KB (20,704 words) - 12:28, 9 January 2024
  • ...an get around this issue by manually clipping the 0-data for the XX and LL polarization with <i>flagdata</i>: Spectral Windows: (1 unique spectral windows and 1 unique polarization setups)
    57 KB (8,166 words) - 15:22, 22 October 2018
  • ...an get around this issue by manually clipping the 0-data for the XX and LL polarization with <i>flagdata</i>: Spectral Windows: (1 unique spectral windows and 1 unique polarization setups)
    53 KB (7,739 words) - 10:46, 25 April 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 ...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 to
    147 KB (20,282 words) - 17:44, 6 December 2022
  • Spectral Windows: (14 unique spectral windows and 1 unique polarization setups) 3) Calculate the weights based on the rms of the cross-polarization products (currently not supported in {{statwt}}).
    42 KB (5,552 words) - 14:34, 6 November 2018
  • ...an get around this issue by manually clipping the 0-data for the XX and LL polarization with <i>flagdata</i>: Spectral Windows: (1 unique spectral windows and 1 unique polarization setups)
    53 KB (7,864 words) - 12:50, 29 September 2020
  • Spectral Windows: (14 unique spectral windows and 1 unique polarization setups) 3) Calculate the weights based on the rms of the cross-polarization products (currently not supported in {{statwt}}).
    44 KB (5,841 words) - 20:00, 23 April 2020
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) ...above plot and the corresponding plots for the other spectral windows and polarization products. The purpose here is to get the phases approximately flat as a fu
    58 KB (8,691 words) - 11:04, 23 November 2011
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) ...above plot and the corresponding plots for the other spectral windows and polarization products. The purpose here is to get the phases approximately flat as a fu
    58 KB (8,728 words) - 17:14, 25 January 2012
  • Spectral Windows: (64 unique spectral windows and 1 unique polarization setups) ...seconds, as a function of antenna index (you will get one for each spw and polarization):
    26 KB (3,524 words) - 10:41, 14 June 2016
  • Spectral Windows: (64 unique spectral windows and 1 unique polarization setups) ...seconds, as a function of antenna index (you will get one for each spw and polarization):
    26 KB (3,524 words) - 13:14, 20 April 2017
  • Spectral Windows: (64 unique spectral windows and 1 unique polarization setups) ...seconds, as a function of antenna index (you will get one for each spw and polarization):
    26 KB (3,524 words) - 11:47, 18 November 2016
  • Spectral Windows: (64 unique spectral windows and 1 unique polarization setups) ...seconds, as a function of antenna index (you will get one for each spw and polarization):
    27 KB (3,594 words) - 18:15, 20 July 2017
  • ...between "G" and "T" (the former generates solutions independently for each polarization, and the latter averages two polarizations before determining the solutions
    15 KB (2,072 words) - 14:42, 12 June 2019
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) ...above plot and the corresponding plots for the other spectral windows and polarization products. The purpose here is to get the phases approximately flat as a fu
    60 KB (9,062 words) - 13:47, 4 September 2012
  • ...an get around this issue by manually clipping the 0-data for the XX and LL polarization with <i>flagdata</i>: Spectral Windows: (1 unique spectral windows and 1 unique polarization setups)
    57 KB (8,502 words) - 18:49, 22 December 2020
  • ...ed spectral windows, centered at 4.6 and 7.5 GHz, and were set up for full polarization calibration. ...shelp NRAO HelpDesk]. We are currently developing a CASAguide specific to polarization in order to address this topic more broadly.
    145 KB (21,313 words) - 19:35, 2 January 2019
  • Spectral Windows: (64 unique spectral windows and 1 unique polarization setups) ...seconds, as a function of antenna index (you will get one for each spw and polarization):
    27 KB (3,654 words) - 14:39, 6 November 2018
  • Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    13 KB (1,838 words) - 17:57, 6 January 2012
  • Spectral Windows: (8 unique spectral windows and 1 unique polarization setups) ...presentative plots are also displayed. Each column displays an individual polarization product; since we're using all four, from left to right are RR, RL, LR, and
    80 KB (11,156 words) - 17:30, 9 May 2014
  • Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    13 KB (1,853 words) - 13:35, 9 January 2012
  • Spectral Windows: (16 unique spectral windows and 1 unique polarization setups)
    14 KB (1,935 words) - 23:52, 10 November 2021
  • Spectral Windows: (8 unique spectral windows and 1 unique polarization setups) ...presentative plots are also displayed. Each column displays an individual polarization product; since we're using all four, from left to right are RR, RL, LR, and
    76 KB (10,592 words) - 15:24, 11 December 2012
  • FEED/ POLARIZATION/ table.dat table.f11_TSM1 table.f5 table.f8_TSM1
    15 KB (2,361 words) - 12:09, 14 December 2018
  • Spectral Windows: (64 unique spectral windows and 1 unique polarization setups) ...seconds, as a function of antenna index (you will get one for each spw and polarization):
    28 KB (3,769 words) - 11:37, 10 July 2019
  • ...an get around this issue by manually clipping the 0-data for the XX and LL polarization with <i>flagdata</i>: Spectral Windows: (1 unique spectral windows and 1 unique polarization setups)
    63 KB (9,411 words) - 23:23, 12 February 2023
  • Spectral Windows: (8 unique spectral windows and 1 unique polarization setups) ...presentative plots are also displayed. Each column displays an individual polarization product; since we're using all four, from left to right are RR, RL, LR, and
    77 KB (10,632 words) - 16:09, 2 May 2013
  • Spectral Windows: (8 unique spectral windows and 1 unique polarization setups) ...presentative plots are also displayed. Each column displays an individual polarization product; since we're using all four, from left to right are RR, RL, LR, and
    77 KB (10,632 words) - 19:57, 4 February 2014
  • ...between "G" and "T" (the former generates solutions independently for each polarization, and the latter averages two polarizations before determining the solutions
    15 KB (2,227 words) - 17:06, 12 October 2023
  • Spectral Windows: (64 unique spectral windows and 1 unique polarization setups) ...seconds, as a function of antenna index (you will get one for each spw and polarization):
    28 KB (3,783 words) - 13:04, 13 November 2020
  • ...d imaging. (See the CASAguide on radio galaxy 3C75 for an introduction to polarization calibration.) * J0319+4130 = 3C 84, which was used as a polarization calibrator; and
    142 KB (20,826 words) - 13:06, 14 July 2020
  • Spectral Windows: (64 unique spectral windows and 1 unique polarization setups) ...seconds, as a function of antenna index (you will get one for each spw and polarization):
    29 KB (3,922 words) - 11:40, 2 May 2022
  • Spectral Windows: (8 unique spectral windows and 1 unique polarization setups) ...presentative plots are also displayed. Each column displays an individual polarization product; since we're using all four, from left to right are RR, RL, LR, and
    77 KB (10,677 words) - 15:29, 14 June 2012
  • Spectral Windows: (8 unique spectral windows and 1 unique polarization setups) ...presentative plots are also displayed. Each column displays an individual polarization product; since we're using all four, from left to right are RR, RL, LR, and
    77 KB (10,677 words) - 13:28, 14 June 2012
  • ...d imaging. (See the CASAguide on radio galaxy 3C75 for an introduction to polarization calibration.) * J0319+4130 = 3C 84, which was used as a polarization calibrator; and
    153 KB (22,510 words) - 11:29, 14 February 2023
  • ...d imaging. (See the CASAguide on radio galaxy 3C75 for an introduction to polarization calibration.) * J0319+4130 = 3C 84, which was used as a polarization calibrator; and
    144 KB (21,056 words) - 15:58, 29 October 2020
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) ...above plot and the corresponding plots for the other spectral windows and polarization products. The purpose here is to get the phases approximately flat as a fu
    61 KB (9,025 words) - 21:41, 6 July 2015
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) ...above plot and the corresponding plots for the other spectral windows and polarization products. The purpose here is to get the phases approximately flat as a fu
    61 KB (9,063 words) - 09:32, 10 April 2017
  • ...imaging. (See the CASA guide on radio galaxy 3C75 for an introduction to polarization calibration.) * J0319+4130 = 3C 84, which was used as a polarization calibrator; and
    154 KB (22,682 words) - 12:13, 1 March 2024
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) ...above plot and the corresponding plots for the other spectral windows and polarization products. The purpose here is to get the phases approximately flat as a fu
    61 KB (9,098 words) - 16:46, 21 October 2020
  • ...ed spectral windows, centered at 4.6 and 7.5 GHz, and were set up for full polarization calibration. ...med to have a precisely known flux density; the spectral bandpass; and the polarization position angle;
    170 KB (25,424 words) - 14:50, 6 June 2017
  • ...ed spectral windows, centered at 4.6 and 7.5 GHz, and were set up for full polarization calibration. ...med to have a precisely known flux density; the spectral bandpass; and the polarization position angle;
    178 KB (26,597 words) - 19:03, 30 October 2018
  • ...ed spectral windows, centered at 4.6 and 7.5 GHz, and were set up for full polarization calibration. ...med to have a precisely known flux density; the spectral bandpass; and the polarization position angle;
    168 KB (25,178 words) - 19:39, 25 August 2016
  • ...an get around this issue by manually clipping the 0-data for the XX and LL polarization with <i>flagdata</i>: Spectral Windows: (1 unique spectral windows and 1 unique polarization setups)
    66 KB (9,867 words) - 13:55, 24 January 2024
  • ...an get around this issue by manually clipping the 0-data for the XX and LL polarization with <i>flagdata</i>: Spectral Windows: (1 unique spectral windows and 1 unique polarization setups)
    66 KB (9,882 words) - 11:21, 29 February 2024
  • ...an get around this issue by manually clipping the 0-data for the XX and LL polarization with <i>flagdata</i>: Spectral Windows: (1 unique spectral windows and 1 unique polarization setups)
    66 KB (9,882 words) - 14:06, 29 February 2024
  • ...ed spectral windows, centered at 4.6 and 7.5 GHz, and were set up for full polarization calibration. ...med to have a precisely known flux density; the spectral bandpass; and the polarization position angle;
    163 KB (24,232 words) - 18:34, 16 July 2015
  • Spectral Windows: (14 unique spectral windows and 1 unique polarization setups) 3) Calculate the weights based on the rms of the cross-polarization products (currently not supported in {{statwt}}).
    42 KB (5,603 words) - 19:31, 12 November 2020
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) Spectral Windows: (6 unique spectral windows and 1 unique polarization setups)
    37 KB (5,642 words) - 19:30, 19 May 2015
  • ...ed spectral windows, centered at 4.6 and 7.5 GHz, and were set up for full polarization calibration. ...med to have a precisely known flux density; the spectral bandpass; and the polarization position angle;
    163 KB (24,302 words) - 18:13, 10 March 2016
  • Spectral Windows: (14 unique spectral windows and 1 unique polarization setups) 3) Calculate the weights based on the rms of the cross-polarization products (currently not supported in [https://casadocs.readthedocs.io/en/v6
    46 KB (6,223 words) - 17:18, 9 August 2021
  • ...e the observations had a full-polarization correlator setup and included a polarization calibrator, for the purposes of this tutorial we will focus on the total in * J0319+4130 = 3C 84, a polarization calibrator (ignored in this tutorial); and
    124 KB (19,290 words) - 12:33, 23 April 2024
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups) Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    48 KB (7,218 words) - 15:07, 23 May 2012
  • Spectral Windows: (8 unique spectral windows and 1 unique polarization setups) ...presentative plots are also displayed. Each column displays an individual polarization product; since we're using all four, from left to right are RR, RL, LR, and
    79 KB (11,069 words) - 23:21, 4 June 2015
  • ...with 0.12 km/s channels (needs to be entered in the field ''bandwidth per polarization'', the '''expected rms noise for the spectral lines is about 32 mJy/beam''' ...like baseline errors and baseline-dependent bandpass errors. Additionally, polarization errors can contribute (which we did not calibrate at all), as well as imper
    41 KB (6,493 words) - 21:20, 23 April 2012
  • ...with 0.12 km/s channels (needs to be entered in the field ''bandwidth per polarization'', the '''expected rms noise for the spectral lines is about 32 mJy/beam''' ...like baseline errors and baseline-dependent bandpass errors. Additionally, polarization errors can contribute (which we did not calibrate at all), as well as imper
    41 KB (6,495 words) - 18:36, 12 January 2012
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) ...op plots are also displayed (Figure 8). Each column displays an individual polarization product; all four polarizations are, from left to right, RR, RL, LR, and LL
    73 KB (9,761 words) - 12:19, 1 August 2017
  • Spectral Windows: (17 unique spectral windows and 2 unique polarization setups) ...e sdplot task. The commands below will plot one spectrum per scan, spw and polarization. It is difficult to describe what a good spectrum looks like at this stage.
    39 KB (4,942 words) - 10:56, 4 August 2014
  • [[Image:X3c1_wvrtsys.intphase_X.png|thumb|<caption>Phase solutions for the X polarization for every integration time of the first dataset.</caption>]] [[Image:X3c1_wvrtsys.scanphase_X.png|thumb|<caption>Phase solutions for the X polarization for each scan of the first dataset.</caption>]]
    49 KB (7,548 words) - 15:38, 9 May 2012
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) [[Image:X3c1_wvrtsys.intphase_X.png|thumb|<caption>Phase solutions for the X polarization for every integration time of the first dataset.</caption>]]
    64 KB (10,004 words) - 16:29, 31 May 2012
  • ...with 0.12 km/s channels (needs to be entered in the field ''bandwidth per polarization''), the '''expected rms noise for the spectral lines is about 32 mJy/beam'' ...like baseline errors and baseline-dependent bandpass errors. Additionally, polarization errors (which we did not calibrate at all) can contribute, as well as imper
    45 KB (6,856 words) - 16:30, 12 June 2012
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) Spectral Windows: (6 unique spectral windows and 1 unique polarization setups)
    37 KB (5,732 words) - 09:33, 10 April 2017
  • Spectral Windows: (8 unique spectral windows and 1 unique polarization setups) ...presentative plots are also displayed. Each column displays an individual polarization product; since we're using all four, from left to right are RR, RL, LR, and
    83 KB (11,246 words) - 12:30, 3 November 2015
  • ...with 0.12 km/s channels (needs to be entered in the field ''bandwidth per polarization''), the '''expected rms noise for the spectral lines is about 32 mJy/beam'' ...like baseline errors and baseline-dependent bandpass errors. Additionally, polarization errors (which we did not calibrate at all) can contribute, as well as imper
    62 KB (9,630 words) - 13:49, 19 December 2012
  • ...with 0.12 km/s channels (needs to be entered in the field ''bandwidth per polarization''), the '''expected rms noise for the spectral lines is about 32 mJy/beam'' ...like baseline errors and baseline-dependent bandpass errors. Additionally, polarization errors (which we did not calibrate at all) can contribute, as well as imper
    63 KB (9,658 words) - 09:46, 18 June 2013
  • ...with 0.12 km/s channels (needs to be entered in the field ''bandwidth per polarization''), the '''expected rms noise for the spectral lines is about 32 mJy/beam'' ...like baseline errors and baseline-dependent bandpass errors. Additionally, polarization errors (which we did not calibrate at all) can contribute, as well as imper
    63 KB (9,660 words) - 14:18, 12 November 2014
  • ...with 0.12 km/s channels (needs to be entered in the field ''bandwidth per polarization''), the '''expected rms noise for the spectral lines is about 32 mJy/beam'' ...like baseline errors and baseline-dependent bandpass errors. Additionally, polarization errors (which we did not calibrate at all) can contribute, as well as imper
    47 KB (7,259 words) - 16:08, 31 May 2012
  • Spectral Windows: (8 unique spectral windows and 1 unique polarization setups) ...presentative plots are also displayed. Each column displays an individual polarization product; since we're using all four, from left to right are RR, RL, LR, and
    71 KB (9,680 words) - 12:37, 9 April 2012
  • ...is page (the final target 3C138, will be released separately with other SV polarization data in the near future).
    16 KB (2,452 words) - 10:11, 8 May 2018
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) [[Image:X3c1_wvrtsys.intphase_X.png|thumb|<caption>Phase solutions for the X polarization for every integration time of the first dataset.</caption>]]
    76 KB (11,820 words) - 10:34, 25 July 2012
  • Spectral Windows: (64 unique spectral windows and 1 unique polarization setups) consists of 128 dual (RR, LL) polarization 1 MHz wide channels, for a
    52 KB (7,692 words) - 16:02, 23 February 2024
  • ...observing personality, using dual polarization with 4 spectral windows per polarization. Each spectral window is has a bandwidth of 64 MHz, and is divided into 12 Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    118 KB (15,469 words) - 10:45, 30 June 2022
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) [[Image:X3c1_wvrtsys.intphase_X.png|thumb|<caption>Phase solutions for the X polarization for every integration time of the first dataset.</caption>]]
    78 KB (12,026 words) - 21:09, 10 December 2013
  • ...observing personality, using dual polarization with 4 spectral windows per polarization. Each spectral window is has a bandwidth of 64 MHz, and is divided into 12 Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    119 KB (15,705 words) - 16:26, 30 April 2024
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) [[Image:X3c1_wvrtsys.intphase_X.png|thumb|<caption>Phase solutions for the X polarization for every integration time of the first dataset.</caption>]]
    78 KB (12,045 words) - 16:58, 7 November 2012
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) Spectral Windows: (6 unique spectral windows and 1 unique polarization setups)
    39 KB (5,971 words) - 14:39, 19 August 2021
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) ...TFCrop plots are displayed (Figure 12). Each column displays an individual polarization product; all four polarizations are, from left to right, RR, RL, LR, and LL
    85 KB (11,750 words) - 19:00, 30 November 2018
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) Spectral Windows: (6 unique spectral windows and 1 unique polarization setups)
    40 KB (6,024 words) - 16:09, 19 August 2021
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) Spectral Windows: (6 unique spectral windows and 1 unique polarization setups)
    40 KB (6,039 words) - 14:44, 19 August 2021
  • ...ds, as a function of antenna index (you will get one for each sub-band and polarization): ...ize of the MS, and will speed up the imaging process. We can also drop the polarization products since they have not been calibrated and will not be used for imagi
    48 KB (7,521 words) - 11:13, 6 April 2016
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) Spectral Windows: (6 unique spectral windows and 1 unique polarization setups)
    40 KB (6,067 words) - 11:49, 7 April 2022
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) [[Image:X3c1_wvrtsys.intphase_X.png|thumb|<caption>Phase solutions for the X polarization for every integration time of the first dataset.</caption>]]
    79 KB (12,189 words) - 16:20, 23 May 2014
  • Spectral Windows: (16 unique spectral windows and 2 unique polarization setups)
    18 KB (2,494 words) - 10:53, 19 September 2019
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) Spectral Windows: (6 unique spectral windows and 1 unique polarization setups)
    41 KB (6,318 words) - 16:11, 19 August 2021
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) ...TFCrop plots are displayed (Figure 12). Each column displays an individual polarization product; all four polarizations are, from left to right, RR, RL, LR, and LL
    83 KB (11,531 words) - 16:50, 5 July 2019
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) ...TFCrop plots are displayed (Figure 12). Each column displays an individual polarization product; all four polarizations are, from left to right, RR, RL, LR, and LL
    83 KB (11,548 words) - 17:50, 9 November 2020
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) ...TFCrop plots are displayed (Figure 12). Each column displays an individual polarization product; all four polarizations are, from left to right, RR, RL, LR, and LL
    87 KB (12,141 words) - 11:38, 2 May 2022
  • [[Image:X3c1_wvrtsys.intphase_X.png|thumb|Phase solutions for the X polarization for every integration time of the first dataset.]] [[Image:X3c1_wvrtsys.scanphase_X.png|thumb|Phase solutions for the X polarization for every for every scan of the first dataset.]]
    60 KB (9,450 words) - 16:45, 23 April 2012
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) ...TFCrop plots are displayed (Figure 12). Each column displays an individual polarization product; all four polarizations are, from left to right, RR, RL, LR, and LL
    87 KB (12,153 words) - 15:20, 13 February 2023
  • As of CASA 5.6, auto-multithresh now functions with polarization data. It applies the same algorithms to the Stokes QUV images as used for t Spectral Windows: (1 unique spectral windows and 1 unique polarization setups)
    42 KB (5,977 words) - 16:32, 8 March 2024
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) ...TFCrop plots are displayed (Figure 12). Each column displays an individual polarization product; all four polarizations are, from left to right, RR, RL, LR, and LL
    87 KB (12,186 words) - 11:56, 1 March 2024
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) ...ve plots are also displayed (Figure 8). Each column displays an individual polarization product; all four polarizations are,from left to right, RR, RL, LR, and LL.
    68 KB (9,089 words) - 18:34, 18 October 2016
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) ...ve plots are also displayed (Figure 8). Each column displays an individual polarization product; all four polarizations are,from left to right, RR, RL, LR, and LL.
    68 KB (9,104 words) - 18:34, 18 October 2016
  • ....aips.nrao.edu/cgi-bin/ZXHLP2.PL?TVFLG TVFLG] will start showing the other polarization.
    63 KB (10,564 words) - 19:14, 1 June 2023
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) ...TFCrop plots are displayed (Figure 12). Each column displays an individual polarization product; all four polarizations are, from left to right, RR, RL, LR, and LL
    88 KB (12,444 words) - 12:57, 30 April 2024
  • ....aips.nrao.edu/cgi-bin/ZXHLP2.PL?TVFLG TVFLG] will start showing the other polarization.
    63 KB (10,611 words) - 13:48, 18 December 2023
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) Spectral Windows: (6 unique spectral windows and 1 unique polarization setups)
    42 KB (6,416 words) - 17:35, 22 April 2024
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) ...op plots are also displayed (Figure 8). Each column displays an individual polarization product; all four polarizations are, from left to right, RR, RL, LR, and LL
    69 KB (9,365 words) - 15:46, 19 July 2017
  • ...with 0.12 km/s channels (needs to be entered in the field ''bandwidth per polarization''), the '''expected rms noise for the spectral lines is about 32 mJy/beam'' ...like baseline errors and baseline-dependent bandpass errors. Additionally, polarization errors (which we did not calibrate at all) can contribute, as well as imper
    63 KB (9,660 words) - 21:36, 6 July 2015
  • ...with 0.12 km/s channels (needs to be entered in the field ''bandwidth per polarization''), the '''expected rms noise for the spectral lines is about 32 mJy/beam'' ...like baseline errors and baseline-dependent bandpass errors. Additionally, polarization errors (which we did not calibrate at all) can contribute, as well as imper
    62 KB (9,547 words) - 17:00, 19 August 2021
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) Spectral Windows: (6 unique spectral windows and 1 unique polarization setups)
    44 KB (6,634 words) - 11:13, 12 October 2023
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    52 KB (8,201 words) - 12:32, 9 April 2012
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    53 KB (8,230 words) - 18:47, 17 May 2012
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups) Spectral Windows: (6 unique spectral windows and 1 unique polarization setups)
    44 KB (6,740 words) - 16:10, 19 August 2021
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    53 KB (8,284 words) - 01:44, 19 January 2012
  • Spectral Windows: (8 unique spectral windows and 1 unique polarization setups) ...presentative plots are also displayed. Each column displays an individual polarization product; since we're using all four, from left to right are RR, RL, LR, and
    72 KB (9,756 words) - 01:45, 19 January 2012
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    94 KB (14,664 words) - 13:42, 5 May 2017
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    28 KB (4,108 words) - 16:24, 9 October 2012
  • ...with 0.12 km/s channels (needs to be entered in the field ''bandwidth per polarization''), the '''expected rms noise for the spectral lines is about 32 mJy/beam'' ...like baseline errors and baseline-dependent bandpass errors. Additionally, polarization errors (which we did not calibrate at all) can contribute, as well as imper
    66 KB (10,129 words) - 15:56, 3 April 2017
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    29 KB (4,266 words) - 17:07, 20 November 2012
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) [[Image:X3c1_wvrtsys.intphase_X.png|thumb|<caption>Phase solutions for the X polarization for every integration time of the first dataset.</caption>]]
    79 KB (12,190 words) - 21:32, 6 July 2015
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) [[Image:X3c1_wvrtsys.intphase_X.png|thumb|<caption>Phase solutions for the X polarization for every integration time of the first dataset.</caption>]]
    78 KB (11,957 words) - 16:55, 19 August 2021
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) ...ations of the phase solutions with {{plotcal}}. We will plot the XX and YY polarization products separately and make different subplots for each of the spectral wi
    67 KB (10,305 words) - 09:50, 10 May 2012
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    29 KB (4,388 words) - 11:43, 12 November 2014
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    30 KB (4,407 words) - 20:48, 10 December 2013
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) [[Image:X3c1_wvrtsys.intphase_X.png|thumb|<caption>Phase solutions for the X polarization for every integration time of the first dataset.</caption>]]
    81 KB (12,419 words) - 09:36, 10 April 2017
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups) Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    66 KB (9,687 words) - 17:49, 15 June 2012
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups) Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    65 KB (9,635 words) - 13:24, 19 November 2012
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    26 KB (3,752 words) - 09:31, 4 April 2017
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    22 KB (2,892 words) - 16:28, 28 February 2024
  • # crowded 1 ➜ to plot all polarization and IFs on top of each other. ...only except it now tells you how it is adjusting the amplitudes in each IF/polarization.
    49 KB (7,800 words) - 17:42, 29 March 2022
  • Spectral Windows: (18 unique spectral windows and 1 unique polarization setups) ...spw 0~7). We will delete this (will also delete LL so there are no orphan polarization products, which would be ignored by {{clean}} in the imaging stage).
    95 KB (12,507 words) - 11:51, 23 May 2012
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups) Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    68 KB (9,999 words) - 11:41, 12 November 2014
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups) Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    68 KB (10,006 words) - 21:13, 10 December 2013
  • As of CASA 5.6, auto-multithresh now functions with polarization data. It applies the same algorithms to the Stokes QUV images as used for t Spectral Windows: (1 unique spectral windows and 1 unique polarization setups)
    54 KB (7,365 words) - 11:29, 3 April 2024
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    23 KB (2,951 words) - 13:49, 7 December 2023
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) ...sets, Antenna DV12 exhibits periodic spikes in Tsys vs. frequency for one polarization (see <xr id="Uid___A002_X215db8_X392.tdm.tsys.3c279.DV11.spw5.CASA3_4.png"/
    101 KB (15,763 words) - 13:48, 5 June 2012
  • Spectral Windows: (18 unique spectral windows and 1 unique polarization setups) ...spw 0~7). We will delete this (will also delete LL so there are no orphan polarization products, which would be ignored by {{clean}} in the imaging stage).
    98 KB (12,933 words) - 17:03, 22 October 2012
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    111 KB (17,150 words) - 09:24, 5 October 2021
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    112 KB (17,190 words) - 12:29, 11 October 2021
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    111 KB (17,130 words) - 07:51, 5 October 2021
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    111 KB (17,131 words) - 10:44, 5 October 2021
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    111 KB (17,131 words) - 10:06, 5 October 2021
  • Spectral Windows: (64 unique spectral windows and 1 unique polarization setups) ...a single baseline (ea02&ea05), channel (31, for all spectral windows), and polarization (RR) versus time. Note that limiting the selected data with appropriate fi
    155 KB (16,512 words) - 00:59, 5 February 2014
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    110 KB (17,076 words) - 13:43, 11 October 2021
  • Spectral Windows: (64 unique spectral windows and 1 unique polarization setups) ...a single baseline (ea02&ea05), channel (31, for all spectral windows), and polarization (RR) versus time. Note that limiting the selected data with appropriate fi
    156 KB (16,716 words) - 13:54, 16 December 2014
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    112 KB (17,278 words) - 14:34, 5 October 2021
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    113 KB (17,396 words) - 16:19, 20 August 2021
  • Spectral Windows: (64 unique spectral windows and 1 unique polarization setups) ...a single baseline (ea02&ea05), channel (31, for all spectral windows), and polarization (RR) versus time. Note that limiting the selected data with appropriate fi
    136 KB (14,700 words) - 19:55, 4 February 2014
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    114 KB (17,595 words) - 15:08, 20 August 2021
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    114 KB (17,621 words) - 16:05, 19 August 2021
  • ...3 INFO listobs Spectral Windows: (5 unique spectral windows and 1 unique polarization setups) ...presentative plots are also displayed. Each column displays an individual polarization product; since we're using all four polarizations, from left to right are R
    89 KB (12,476 words) - 10:49, 12 April 2016
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    114 KB (17,545 words) - 13:03, 24 October 2022
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    114 KB (17,545 words) - 10:35, 25 August 2022
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    114 KB (17,557 words) - 14:43, 20 August 2021
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    29 KB (4,388 words) - 21:53, 6 July 2015
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    30 KB (4,388 words) - 11:03, 21 February 2018
  • Spectral Windows: (16 unique spectral windows and 1 unique polarization setups) ...igure 6: The phase solutions vs. time for the first 9 antennas, colored by polarization.]]
    86 KB (13,200 words) - 15:40, 18 October 2020
  • ...3 INFO listobs Spectral Windows: (5 unique spectral windows and 1 unique polarization setups) ...presentative plots are also displayed. Each column displays an individual polarization product; since we're using all four polarizations, from left to right are R
    94 KB (13,350 words) - 17:09, 13 April 2016
  • Spectral Windows: (9 unique spectral windows and 2 unique polarization setups) Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    118 KB (17,944 words) - 14:22, 17 April 2024
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups) Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    68 KB (9,999 words) - 13:32, 12 September 2017
  • Spectral Windows: (16 unique spectral windows and 1 unique polarization setups) ...igure 6: The phase solutions vs. time for the first 9 antennas, colored by polarization.]]
    94 KB (14,384 words) - 17:33, 20 July 2021
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups) Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    68 KB (10,027 words) - 13:15, 4 April 2017
  • Spectral Windows: (18 unique spectral windows and 1 unique polarization setups) ...spw 0~7). We will delete this (will also delete LL so there are no orphan polarization products, which would be ignored by {{clean}} in the imaging stage).
    114 KB (15,222 words) - 16:13, 9 November 2012
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups) Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    68 KB (9,999 words) - 21:50, 6 July 2015
  • Spectral Windows: (18 unique spectral windows and 1 unique polarization setups) ...spw 0~7). We will delete this (will also delete LL so there are no orphan polarization products, which would be ignored by {{clean}} in the imaging stage).
    114 KB (15,237 words) - 20:04, 4 February 2014
  • Spectral Windows: (18 unique spectral windows and 1 unique polarization setups) ...spw 0~7). We will delete this (will also delete LL so there are no orphan polarization products, which would be ignored by {{clean}} in the imaging stage).
    115 KB (15,378 words) - 19:52, 4 February 2014
  • Spectral Windows: (18 unique spectral windows and 1 unique polarization setups) ...spw 0~7). We will delete this (will also delete LL so there are no orphan polarization products, which would be ignored by {{clean}} in the imaging stage).
    115 KB (15,378 words) - 19:51, 4 February 2014
  • Spectral Windows: (18 unique spectral windows and 1 unique polarization setups) ...spw 0~7). We will delete this (will also delete LL so there are no orphan polarization products, which would be ignored by {{clean}} in the imaging stage).
    93 KB (12,148 words) - 18:33, 27 January 2012
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups) Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    69 KB (10,222 words) - 15:51, 12 September 2017
  • Spectral Windows: (18 unique spectral windows and 1 unique polarization setups) ...spw 0~7). We will delete this (will also delete LL so there are no orphan polarization products, which would be ignored by {{clean}} in the imaging stage).
    94 KB (12,292 words) - 01:44, 19 January 2012
  • Spectral Windows: (18 unique spectral windows and 1 unique polarization setups) ...spw 0~7). We will delete this (will also delete LL so there are no orphan polarization products, which would be ignored by {{clean}} in the imaging stage).
    117 KB (15,635 words) - 13:17, 6 February 2014
  • Spectral Windows: (18 unique spectral windows and 1 unique polarization setups) ...spw 0~7). We will delete this (will also delete LL so there are no orphan polarization products, which would be ignored by {{clean}} in the imaging stage).
    117 KB (15,635 words) - 13:53, 16 December 2014
  • Spectral Windows: (16 unique spectral windows and 1 unique polarization setups) ...igure 6: The phase solutions vs. time for the first 9 antennas, colored by polarization.]]
    91 KB (13,780 words) - 12:03, 2 April 2024
  • Spectral Windows: (14 unique spectral windows and 1 unique polarization setups)
    27 KB (3,372 words) - 18:44, 27 October 2021
  • Spectral Windows: (64 unique spectral windows and 1 unique polarization setups) ...a single baseline (ea02&ea05), channel (31, for all spectral windows), and polarization (RR) versus time. Note that limiting the selected data with appropriate fi
    155 KB (16,800 words) - 23:15, 4 June 2015
  • Spectral Windows: (64 unique spectral windows and 1 unique polarization setups) ...a single baseline (ea02&ea05), channel (31, for all spectral windows), and polarization (RR) versus time. Note that limiting the selected data with appropriate fi
    155 KB (16,783 words) - 15:49, 13 April 2016
  • ...vity-calculator ALMA sensitivity calculator], a bandwidth of 10 km/s, dual polarization, 12 antennas, and the time on a single pointing of about 300s yields an rms
    41 KB (6,416 words) - 16:05, 16 May 2012
  • ...vity-calculator ALMA sensitivity calculator], a bandwidth of 10 km/s, dual polarization, 12 antennas, and the time on a single pointing of about 300s yields an rms
    40 KB (6,363 words) - 12:47, 5 June 2012
  • Spectral Windows:(24 unique spectral windows and 1 unique polarization setups)
    41 KB (5,906 words) - 11:46, 18 May 2011
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    108 KB (16,739 words) - 15:08, 15 October 2020
  • Spectral Windows: (14 unique spectral windows and 1 unique polarization setups)
    29 KB (3,669 words) - 18:03, 28 July 2017
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    108 KB (16,776 words) - 15:14, 15 October 2020
  • Spectral Windows:(24 unique spectral windows and 1 unique polarization setups)
    42 KB (6,040 words) - 13:25, 5 May 2011
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups) Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    76 KB (10,842 words) - 12:32, 10 June 2021
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups) Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    76 KB (10,827 words) - 11:54, 25 October 2022
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups) Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    77 KB (10,929 words) - 09:22, 28 September 2018
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups) Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    76 KB (10,829 words) - 11:00, 8 September 2022
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups) Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    76 KB (10,829 words) - 09:40, 27 October 2022
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups) Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    78 KB (11,090 words) - 15:48, 11 March 2021
  • Spectral Windows: (3 unique spectral windows and 1 unique polarization setups)
    37 KB (5,752 words) - 17:27, 26 May 2011
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    119 KB (18,324 words) - 12:17, 24 February 2023
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    119 KB (18,324 words) - 14:03, 2 March 2023
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups) Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    76 KB (10,831 words) - 08:38, 6 October 2023
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    36 KB (5,365 words) - 10:23, 28 September 2018
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    36 KB (5,329 words) - 11:03, 27 October 2020
  • '''stokes:''' The Stokes polarization to be produced, we want Stokes I.
    36 KB (5,572 words) - 16:38, 30 October 2018
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    37 KB (5,453 words) - 16:43, 11 March 2021
  • Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    44 KB (6,777 words) - 12:19, 19 May 2010
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    37 KB (5,464 words) - 11:16, 10 June 2021
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    81 KB (12,845 words) - 16:03, 1 June 2012
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    81 KB (12,853 words) - 22:34, 6 December 2012
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups) Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    79 KB (11,275 words) - 14:26, 10 June 2021
  • Spectral Windows: (3 unique spectral windows and 1 unique polarization setups)
    39 KB (6,041 words) - 13:04, 5 July 2011
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    37 KB (5,482 words) - 16:40, 10 June 2021
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    37 KB (5,511 words) - 10:16, 7 April 2022
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    37 KB (5,507 words) - 14:15, 25 October 2022
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    37 KB (5,511 words) - 14:16, 25 October 2022
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations. Setting ver Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    79 KB (10,809 words) - 14:21, 9 April 2021
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    82 KB (13,029 words) - 16:14, 30 May 2013
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations. Setting ver Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    79 KB (10,810 words) - 18:24, 14 February 2020
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations. Setting ver Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    85 KB (11,808 words) - 11:37, 2 May 2022
  • '''stokes:''' the Stokes polarization to be calculated; we want Stokes ''I''.
    39 KB (5,805 words) - 14:55, 19 March 2019
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    38 KB (5,651 words) - 08:54, 23 October 2023
  • Spectral Windows: (14 unique spectral windows and 1 unique polarization setups)
    34 KB (4,087 words) - 10:49, 26 January 2023
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    82 KB (12,857 words) - 13:35, 2 June 2015
  • Spectral Windows: (18 unique spectral windows and 1 unique polarization setups) ...spw 0~7). We will delete this (will also delete LL so there are no orphan polarization products, which would be ignored by {{clean}} in the imaging stage).
    125 KB (15,910 words) - 23:10, 4 June 2015
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    84 KB (13,072 words) - 21:45, 25 April 2013
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    83 KB (13,072 words) - 19:38, 4 February 2014
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    84 KB (13,082 words) - 17:15, 5 February 2014
  • Spectral Windows: (18 unique spectral windows and 1 unique polarization setups) ...spw 0~7). We will delete this (will also delete LL so there are no orphan polarization products, which would be ignored by {{clean}} in the imaging stage).
    127 KB (16,188 words) - 17:52, 13 July 2015
  • '''stokes:''' the Stokes polarization to be calculated; we want Stokes ''I''.
    40 KB (6,025 words) - 13:01, 7 June 2019
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations. Setting ver Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    91 KB (12,686 words) - 20:32, 20 February 2024
  • ...and correlator setup (frequencies, bandwidths, channel number and widths, polarization products). Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    134 KB (19,330 words) - 16:53, 29 September 2023
  • Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    45 KB (7,121 words) - 14:11, 21 May 2012
  • '''stokes:''' the Stokes polarization to be calculated; we want Stokes ''I''.
    44 KB (6,627 words) - 13:03, 13 July 2021
  • '''stokes:''' the Stokes polarization to be calculated; we want Stokes ''I''.
    40 KB (6,085 words) - 22:49, 12 November 2020
  • ...vity-calculator ALMA sensitivity calculator], a bandwidth of 10 km/s, dual polarization, 12 antennas, and the time on a single pointing of about 300s yields an rms
    44 KB (6,765 words) - 13:59, 11 October 2021
  • ...vity-calculator ALMA sensitivity calculator], a bandwidth of 10 km/s, dual polarization, 12 antennas, and the time on a single pointing of about 300s yields an rms
    44 KB (6,844 words) - 15:05, 5 October 2021
  • ...vity-calculator ALMA sensitivity calculator], a bandwidth of 10 km/s, dual polarization, 12 antennas, and the time on a single pointing of about 300s yields an rms
    44 KB (6,859 words) - 08:10, 5 October 2021
  • ...vity-calculator ALMA sensitivity calculator], a bandwidth of 10 km/s, dual polarization, 12 antennas, and the time on a single pointing of about 300s yields an rms
    44 KB (6,858 words) - 10:48, 5 October 2021
  • ...vity-calculator ALMA sensitivity calculator], a bandwidth of 10 km/s, dual polarization, 12 antennas, and the time on a single pointing of about 300s yields an rms
    44 KB (6,858 words) - 10:34, 5 October 2021
  • ...vity-calculator ALMA sensitivity calculator], a bandwidth of 10 km/s, dual polarization, 12 antennas, and the time on a single pointing of about 300s yields an rms
    44 KB (6,883 words) - 07:26, 5 October 2021
  • ...vity-calculator ALMA sensitivity calculator], a bandwidth of 10 km/s, dual polarization, 12 antennas, and the time on a single pointing of about 300s yields an rms
    44 KB (6,883 words) - 09:40, 5 October 2021
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    108 KB (16,694 words) - 10:46, 11 June 2019
  • '''stokes:''' the Stokes polarization to be calculated; we want Stokes ''I''.
    45 KB (6,774 words) - 15:57, 27 January 2023
  • Spectral Windows: (14 unique spectral windows and 1 unique polarization setups)
    39 KB (4,613 words) - 17:21, 26 February 2024
  • '''stokes:''' the Stokes polarization to be calculated; we want Stokes ''I''.
    46 KB (6,895 words) - 14:39, 28 February 2024
  • ...49 INFO listobs Spectral Windows: (1 unique spectral windows and 1 unique polarization setups) ...17 INFO listobs Spectral Windows: (1 unique spectral windows and 1 unique polarization setups)
    87 KB (10,559 words) - 13:08, 13 February 2023
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups)
    39 KB (5,284 words) - 16:07, 19 August 2021
  • Spectral Windows: (37 unique spectral windows and 2 unique polarization setups)
    40 KB (4,408 words) - 16:31, 19 August 2021
  • Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    49 KB (7,632 words) - 21:16, 29 August 2011
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups)
    40 KB (5,491 words) - 11:39, 7 April 2022
  • Spectral Windows: (1 unique spectral windows and 1 unique polarization setups)
    37 KB (5,195 words) - 14:44, 12 June 2019
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups)
    39 KB (5,356 words) - 14:36, 19 August 2021
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups)
    40 KB (5,491 words) - 11:06, 12 October 2023
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups)
    40 KB (5,472 words) - 16:52, 2 February 2024
  • Spectral Windows: (37 unique spectral windows and 2 unique polarization setups)
    41 KB (4,534 words) - 08:50, 11 January 2018
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups)
    40 KB (5,435 words) - 14:37, 19 August 2021
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups)
    39 KB (5,283 words) - 01:21, 23 August 2017
  • ...vity-calculator ALMA sensitivity calculator], a bandwidth of 10 km/s, dual polarization, 12 antennas, and the time on a single pointing of about 300s yields an rms
    47 KB (7,341 words) - 16:35, 20 August 2021
  • Spectral Windows: (1 unique spectral windows and 1 unique polarization setups)
    37 KB (5,389 words) - 11:08, 5 March 2018
  • ...vity-calculator ALMA sensitivity calculator], a bandwidth of 10 km/s, dual polarization, 12 antennas, and the time on a single pointing of about 300s yields an rms
    48 KB (7,478 words) - 15:24, 20 August 2021
  • ...vity-calculator ALMA sensitivity calculator], a bandwidth of 10 km/s, dual polarization, 12 antennas, and the time on a single pointing of about 300s yields an rms
    49 KB (7,485 words) - 15:44, 20 August 2021
  • ...vity-calculator ALMA sensitivity calculator], a bandwidth of 10 km/s, dual polarization, 12 antennas, and the time on a single pointing of about 300s yields an rms
    49 KB (7,492 words) - 13:22, 13 October 2021
  • ...vity-calculator ALMA sensitivity calculator], a bandwidth of 10 km/s, dual polarization, 12 antennas, and the time on a single pointing of about 300s yields an rms
    49 KB (7,524 words) - 11:23, 7 April 2022
  • ...vity-calculator ALMA sensitivity calculator], a bandwidth of 10 km/s, dual polarization, 12 antennas, and the time on a single pointing of about 300s yields an rms
    49 KB (7,509 words) - 00:55, 31 December 2023
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    84 KB (13,101 words) - 13:57, 3 November 2015
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    83 KB (13,039 words) - 18:00, 20 July 2015
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations. Setting ver Spectral Windows: (1 unique spectral windows and 1 unique polarization setups)
    94 KB (13,008 words) - 20:51, 31 January 2023
  • Spectral Windows: (1 unique spectral windows and 1 unique polarization setups)
    41 KB (5,884 words) - 16:03, 4 May 2022
  • Spectral Windows: (1 unique spectral windows and 1 unique polarization setups)
    41 KB (5,881 words) - 13:28, 1 May 2023
  • Spectral Windows: (1 unique spectral windows and 1 unique polarization setups)
    42 KB (6,001 words) - 17:01, 12 October 2023
  • ...vity-calculator ALMA sensitivity calculator], a bandwidth of 10 km/s, dual polarization, 12 antennas, and the time on a single pointing of about 300s yields an rms
    51 KB (7,819 words) - 15:29, 29 February 2024
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    90 KB (14,142 words) - 18:38, 10 March 2016
  • Spectral Windows: (1 unique spectral windows and 1 unique polarization setups)
    42 KB (6,134 words) - 12:18, 15 December 2023
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    92 KB (14,512 words) - 17:26, 25 May 2017
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    92 KB (14,496 words) - 16:50, 7 November 2016
  • Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)
    46 KB (7,223 words) - 15:03, 7 September 2023
  • ...h as correlator setup (frequencies, bandwidths, channel number and widths, polarization products), sources, scans, scan intents, and antenna locations: Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    98 KB (15,214 words) - 11:44, 3 October 2018
  • Spectral Windows: (25 unique spectral windows and 2 unique polarization setups)
    49 KB (6,272 words) - 16:27, 26 August 2015
  • Spectral Windows: (37 unique spectral windows and 2 unique polarization setups)
    50 KB (5,729 words) - 12:35, 22 April 2024
  • * ''stokes='I''': since we have not done any polarization calibration, we only create a total-intensity image. For using CLEAN while
    60 KB (9,464 words) - 18:16, 25 May 2016
  • * ''stokes='I''': since we have not done any polarization calibration, we only create a total-intensity image. For using CLEAN while
    60 KB (9,489 words) - 15:18, 25 May 2016
  • * ''stokes='I''': since we have not done any polarization calibration, we only create a total-intensity image. For using CLEAN while
    63 KB (9,901 words) - 16:09, 10 June 2019
  • * ''stokes='I''': since we have not done any polarization calibration, we only create a total-intensity image. For using {{tclean}} w
    64 KB (9,998 words) - 12:51, 11 July 2019
  • * ''stokes='I''': since we have not done any polarization calibration, we only create a total-intensity image. For using CLEAN while
    65 KB (10,257 words) - 13:13, 20 April 2017
  • * ''stokes='I''': since we have not done any polarization calibration, we only create a total-intensity image. For using CLEAN while
    65 KB (10,334 words) - 15:11, 5 October 2017
  • * ''stokes='I''': since we have not done any polarization calibration, we only create a total-intensity image. For using [https://cas
    71 KB (11,202 words) - 16:08, 25 April 2022
  • * ''stokes='I''': since we have not done any polarization calibration, we only create a total-intensity image. For using {{tclean}} w
    66 KB (10,403 words) - 16:09, 7 October 2020
  • * ''stokes='I''': since we have not done any polarization calibration, we only create a total-intensity image. For using [https://cas
    75 KB (11,832 words) - 14:03, 7 February 2023
  • * ''stokes='I''': since we have not done any polarization calibration, we only create a total-intensity image. For using [https://cas
    77 KB (12,054 words) - 13:56, 1 March 2024
  • Spectral Windows: (24 unique spectral windows and 1 unique polarization setups)
    128 KB (15,855 words) - 12:38, 25 November 2014