Search results

• Simulating Observations in CASA 3.3
  ...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
• JuergensSandbox
  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
• EVLA Advanced Topics 3C391 CASA 4.2
  ...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
• Advanced Topics 3C391 - CASA4.2
  ...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
• Simulating Observations in CASA 3.1
  ...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
• Plotbandpass
  ...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
• EVLA Advanced Topics 3C391-CASA4.1
  ...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
• Advanced Topics 3C391 - CASA4.1
  ...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
• EVLA Advanced Topics 3C391
  ...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
• EVLA Advanced Topics 3C391-CASA4.3
  ...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
• EVLA Advanced Topics 3C391-CASA4.4
  ...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
• EVLA Advanced Topics 3C391-CASA4.0
  ...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
• EVLA Advanced Topics 3C391-CASA3.4
  ...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
• P-band basic data reduction path for continuum stokes I imaging
  * 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
• CASA Guides:ATCA Advanced Continuum Polarization Tutorial NGC612-CASA4.7
  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
• Modify Model
  ...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
• ALMAguides old
  * [[3C286_Polarization]]: Demonstration of the reduction of ALMA continuum polarization toward the quasar 3C286
  6 KB (859 words) - 16:29, 8 January 2018
• ALMA SIS14 apcal
  * 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
• Simulating Observations in CASA 4.1
  ...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

View (previous 20 | next 20) (20 | 50 | 100 | 250 | 500)