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- ...ides.nrao.edu/index.php/Simulating_Observations_in_CASA_5.1 Simulations in CASA] section of the CASAguides. ...r all of our simulations. The image center can also be determined with the CASA viewer. Given that the VLA primary beams at the VLA frequencies are much la36 KB (5,572 words) - 16:38, 30 October 2018
- The currently maintained combination CASAguide, written for CASA 4.3.0, can be found here: https://casaguides.nrao.edu/index.php/M100_Band3_ ...ethods to correct the data weights for data reduced in earlier versions of CASA.37 KB (5,732 words) - 09:33, 10 April 2017
- ...tutorial is to provide a first look at imaging ALMA data for those new to CASA. ...4, and possibly earlier versions. The task {{tclean}} is only available in CASA 4.7 and later.37 KB (5,195 words) - 14:44, 12 June 2019
- ...uide is for Version 6.6.3 of CASA.</b> If you are using a later version of CASA and this is the most recent available guide, then you should be able to use This CASA Guide describes the procedure for calibrating a phase-referenced VLBA obser52 KB (8,358 words) - 18:00, 14 May 2024
- ...ides.nrao.edu/index.php/Simulating_Observations_in_CASA_5.1 Simulations in CASA] section of the CASAguides. ...r all of our simulations. The image center can also be determined with the CASA viewer. Given that the VLA primary beams at the VLA frequencies are much la39 KB (5,805 words) - 14:55, 19 March 2019
- ...ge describes the data and introduces the scripts. It is not a full-fledged CASA guide, only background for the hands on portion of the workshop. For the im * Remember that each CASA Measurement Set contains the raw data, corrected data, and a model. Concept9 KB (1,578 words) - 10:49, 27 February 2013
- 3. There is a report that CASA v.4.2.2 may have a bug which makes interactive clean starting from a mask i3 KB (544 words) - 11:41, 9 July 2015
- '''This guide is written for CASA 6.2 and uses Python 3.''' ...ethods to correct the data weights for data reduced in earlier versions of CASA.40 KB (6,067 words) - 11:49, 7 April 2022
- ...and uses Python 3. The same functionality is implemented in Python 2 using CASA 5.7 at [https://casaguides.nrao.edu/index.php?title=M100_Band3_Combine_5.7 ...ethods to correct the data weights for data reduced in earlier versions of CASA.40 KB (6,039 words) - 14:44, 19 August 2021
- This portion of the '''[[NGC3256Band3]]''' CASA Guide will cover the calibration of the raw visibility data. To skip to th # In a terminal outside CASA58 KB (8,691 words) - 11:04, 23 November 2011
- This portion of the '''[[NGC3256Band3]]''' CASA Guide will cover the calibration of the raw visibility data. To skip to th ...designed for CASA 3.4 (≥r19874). If you are using an older version of CASA please see [[TWHydraBand7_Calibration_for_CASA_3.3]].60 KB (9,062 words) - 13:47, 4 September 2012
- ...ethods to correct the data weights for data reduced in earlier versions of CASA. ...e that the imaging presented in this Guide uses the new calibration (using CASA 4.3)39 KB (5,971 words) - 14:39, 19 August 2021
- ...ethods to correct the data weights for data reduced in earlier versions of CASA. ...e that the imaging presented in this Guide uses the new calibration (using CASA 4.3)40 KB (6,024 words) - 16:09, 19 August 2021
- This portion of the '''[[NGC3256Band3 (Caltech)]]''' CASA Guide will cover the calibration of the raw visibility data. To skip to th # In a terminal outside CASA58 KB (8,728 words) - 17:14, 25 January 2012
- This portion of the '''[[NGC3256Band3]]''' CASA Guide will cover the calibration of the raw visibility data. To skip to th '''This guide is designed for CASA 4.1. If you are using an older version of CASA please see [[NGC3256_Band3_Calibration_for_CASA_4.0]].61 KB (9,010 words) - 10:28, 18 April 2013
- ''This CASA Guide is for Version 6.4.1 of CASA, and was last checked with CASA 6.5.4.'' ...://casa.nrao.edu/Data/EVLA/combination/VLA-combination-W49A.tar.gz https://casa.nrao.edu/Data/EVLA/combination/VLA-combination-W49A.tar.gz] (3.0G)30 KB (3,847 words) - 16:55, 22 February 2024
- ...hp?title=EVLA_high_frequency_Spectral_Line_tutorial_-_IRC%2B10216_CASA3.4 CASA 3.4 version] ...as with Ka-band receivers, and select only spectral windows (called spw in CASA) with Ka-band data. This produces a significantly smaller dataset for proce53 KB (8,230 words) - 18:47, 17 May 2012
- libraries. These are third party routines packaged with CASA that allow efficient definition and manipulation of matrices (or images or ...then you will need to [http://www.scipy.org/ download and install numpy]. CASA includes numpy as pat of its basic distribution but keeps it as a separate19 KB (3,193 words) - 18:51, 1 November 2011
- This portion of the '''[[NGC3256Band3]]''' CASA Guide will cover the calibration of the raw visibility data. To skip to th '''This guide is designed for CASA 4.2. If you are using an older version of CASA please see [[NGC3256_Band3_Calibration_for_CASA_4.1]].61 KB (9,025 words) - 11:19, 29 November 2013
- ...and uses Python 3. The same functionality is implemented in Python 2 using CASA 5.7 at [[AntennaeBand7 Imaging 5.7]]''' ...This guide is designed for CASA 6.1. If you are using an older version of CASA please see [[AntennaeBand7]] for earlier versions of this CASAguide.49 KB (7,492 words) - 13:22, 13 October 2021
