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• PlotSunDuringTrack
  This page documents the plotSunDuringTrack function of Python module [[Analysis Utili CASA <2>: au.plotSunDuringTrack(asdm='uid___A002_X54d35d_X761',plotfile=True)
  942 bytes (156 words) - 01:04, 27 January 2013
• Instructions for Authors
  y = 2 y = 2
  3 KB (421 words) - 13:27, 29 August 2011
• Selecting Spectral Windows and Channels
  spw = '0~3' # Spectral windows 0, 1, 2, and 3 ...'2:5~15;25~35' # Channels 5--15 and 25--35 for spectral window 2
  2 KB (296 words) - 15:42, 20 August 2012
• List of All Tutorials
  ==='''[[ ALMAguides | ALMA Guides Main Page]] '''=== ==='''[[ EVLA Tutorials | EVLA Guides Main Page]] '''===
  8 KB (970 words) - 16:45, 10 June 2013
• Protoplanetary Disk Simulation (CASA 4.1)
  * '''To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].''' ...[http://casaguides.nrao.edu/index.php?title=Sim_Inputs Simulation Inputs] page for this and other sample images. ''If you use this FITS data for anything
  5 KB (819 words) - 12:15, 11 June 2013
• Protoplanetary Disk Simulation (CASA 4.0)
  * '''To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].''' ...[http://casaguides.nrao.edu/index.php?title=Sim_Inputs Simulation Inputs] page for this and other sample images. ''If you use this FITS data for anything
  5 KB (807 words) - 14:27, 9 November 2012
• Protoplanetary Disk Simulation (CASA 4.2)
  ...are recommended to begin with the [[Simulation Guide for New Users (CASA 4.2)]].''' * '''This guide is applicable to CASA version 4.2. For older versions of CASA see [[PPdisk_simdata_(CASA_4.1)]].'''
  6 KB (840 words) - 11:06, 25 October 2013
• Extracting data from MIRIAD
  ...a description of how to use the CARMA filler routine will be added to this page. 2. You are running the MIRIAD commands shown on this page in a shell script (csh), with a number of variables defined at the top of y
  4 KB (730 words) - 14:46, 14 May 2010
• Plotweather
  This page documents the '''plotWeather''' function of Python module [[Analysis Utilit empty list means to plot all data from up to 2 of the stations present in the data, which
  1 KB (189 words) - 12:16, 18 January 2013
• PlanetPlots
  This page documents the '''planetPlots''' function of Python module [[Analysis Utilit page per object, where rows are configurations and columns are frequencies.
  3 KB (477 words) - 12:36, 6 September 2013
• Simulating Observations in CASA 5.4
  This page contains tutorials on how to simulate data in CASA. The two main CASA tasks <!-- [[Simulating_Observations_in_CASA_4.2]] -->
  7 KB (1,016 words) - 12:22, 21 March 2024
• Simulating Observations in CASA 6.5.4
  This page contains tutorials on how to simulate data in CASA. The two main CASA tasks [[Simulating Observations in_CASA_4.2]]
  6 KB (922 words) - 18:37, 26 March 2024
• TWHydraBand7 for CASA 3.4 defunct
  '''This page is under construction.''' ...nd7.jpg|thumb|SMA CO(3-2) emission from TW Hya (Hughes et al. 2011; Figure 2).]]
  7 KB (1,192 words) - 12:47, 23 April 2012
• Simulating Observations in CASA 6
  This page contains tutorials on how to simulate data in CASA. The two main CASA tasks ...u/index.php/Simulating_Observations_in_CASA_4.2 Simulation pages in CASA 4.2]. -->
  7 KB (1,115 words) - 16:25, 12 February 2024
• TWHydraBand7 For CASA 3.4
  * '''This page is under construction.''' ...nd7.jpg|thumb|SMA CO(3-2) emission from TW Hya (Hughes et al. 2011; Figure 2).]]
  7 KB (1,210 words) - 13:09, 23 April 2012
• Simulating Observations in CASA 5.1
  This page contains tutorials on how to simulate data in CASA. The two main CASA tasks ...u/index.php/Simulating_Observations_in_CASA_4.2 Simulation pages in CASA 4.2].
  8 KB (1,252 words) - 17:23, 15 February 2023
• Obslist
  This page documents the obslist function of Python module [[Analysis Utilities|analys Antenna 2 = DV07 on pad J510, lat/long offset (m) = -0.3652/ -512.3043
  3 KB (499 words) - 16:45, 4 January 2012
• Simulating Observations in CASA 3.2
  <font color="red">This page is valid for CASA version 3.2. For CASA 3.3, see [[Simulating Observations in CASA 3.3]]. For earlier v ...t>sm</tt> C++ <tt>tool</tt>. The task interface turns a model of the sky (2 to 4 dimensions including frequency and Stokes) into the visibilities that
  8 KB (1,321 words) - 14:34, 1 November 2011
• TWHydraBand7 SS12 Overview
  ...focused on calibration and the afternoon will be focused on imaging. This page gives an introduction to the target and scientific motivation for the obser ...nd7.jpg|thumb|SMA CO(3-2) emission from TW Hya (Hughes et al. 2011; Figure 2).]]
  9 KB (1,497 words) - 11:22, 29 May 2012
• Plotmosaic
  This page documents the '''plotmosaic''' function of Python module [[Analysis Utiliti *au.plotmosaic(vis, sourceid=2, figfile='mosaic.png', coord='relative', skipsource=-1, doplot=True, help=F
  3 KB (468 words) - 09:47, 12 April 2014
• N891 simdata2
  ''A new version of this page exists for CASA 3.3: [[N891 simdata (CASA 3.3)]].'' Jy/Sr = 2x10²³ k T / &lambda;²,
  4 KB (609 words) - 10:38, 4 November 2011
• TWHydraBand7 For CASA 3.3
  ...nd7.jpg|thumb|SMA CO(3-2) emission from TW Hya (Hughes et al. 2011; Figure 2).]] ...Op3_2.gif|thumb|SMA HCO+(3-2) emission from TW Hya (Qi et al. 2008; Figure 2).]]
  7 KB (1,195 words) - 12:49, 23 April 2012
• Protoplanetary Disk Simulation (CASA 4.3)
  <!-- For older versions of CASA see [[Protoplanetary_Disk_Simulation_(CASA_4.2)]].''' --> * '''To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].'''
  6 KB (843 words) - 17:30, 14 December 2018
• Protoplanetary Disk Simulation (CASA 4.4)
  * '''To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].''' ...[http://casaguides.nrao.edu/index.php?title=Sim_Inputs Simulation Inputs] page for this and other sample images. ''If you use this FITS data for anything
  6 KB (841 words) - 18:25, 6 July 2015
• Protoplanetary Disk Simulation (CASA 5.1)
  * '''To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].''' ...[http://casaguides.nrao.edu/index.php?title=Sim_Inputs Simulation Inputs] page for this and other sample images. ''If you use this FITS data for anything
  6 KB (856 words) - 17:39, 14 December 2018
• Protoplanetary Disk Simulation (CASA 5.4)
  * '''To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].''' ...[http://casaguides.nrao.edu/index.php?title=Sim_Inputs Simulation Inputs] page for this and other sample images. ''If you use this FITS data for anything
  6 KB (856 words) - 17:46, 14 December 2018
• AntennaeBand7 North SS12
  on imaging. This page gives an introduction to the target and scientific ...respond to the CO(1-0) intensity map in Wilson et al. (2000; see also Fig. 2). (Credit: NASA, ESA, and the Hubble Heritage Team STScI/AURA-ESA/Hubble Co
  9 KB (1,381 words) - 10:20, 5 June 2012
• Protoplanetary Disk Simulation (CASA 3.4)
  * '''To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].''' # Divide the first two elements of axesLength by 2.
  5 KB (775 words) - 15:37, 12 June 2012
• PPdisk simdata (CASA 4.0)
  * '''To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].''' # Divide the first two elements of axesLength by 2.
  5 KB (775 words) - 12:44, 31 October 2012
• TWHydraBand7 (Caltech)
  ...nd7.jpg|thumb|SMA CO(3-2) emission from TW Hya (Hughes et al. 2011; Figure 2).]] ...Op3_2.gif|thumb|SMA HCO+(3-2) emission from TW Hya (Qi et al. 2008; Figure 2).]]
  8 KB (1,300 words) - 01:45, 19 January 2012
• N891 simdata (CASA 3.3)
  To create a script of the Python code on this page see [[Extracting scripts from these tutorials]]. ...;², <!-- <math>\frac{Jy}{Sr} = \frac{2\times 10^{23} k T}{\pi D^2 \Omega}</math>, where <math>\Omega</math> is the beam solid angle --> = 4x1
  4 KB (739 words) - 11:19, 22 November 2011
• Simulating Observations in CASA 3.1
  ...t>sm</tt> C++ <tt>tool</tt>. The task interface turns a model of the sky (2 to 4 dimensions including frequency and Stokes) into the visibilities that ...3.1.0</font>: The <tt>simdata</tt> task is the task formerly known in 3.0.2 as <tt>simdata2</tt>. The old version of simdata has been removed.
  10 KB (1,479 words) - 13:28, 30 April 2011
• Importing M99
  ...a description of how to use the CARMA filler routine will be added to this page. 2. You are running the MIRIAD commands shown on this page in a shell script (csh), with a number of variables defined at the top of y
  6 KB (980 words) - 10:15, 29 April 2010
• Check for the CASA Incremental Storage Manager Flagging Bug
  An issue in CASA 4.2.1 and earlier has been discovered with the CASA (2) The number of integrations per scan is large
  4 KB (598 words) - 18:21, 4 December 2014
• TWHydraBand7
  ...nd7.jpg|thumb|SMA CO(3-2) emission from TW Hya (Hughes et al. 2011; Figure 2).]] ...Op3_2.gif|thumb|SMA HCO+(3-2) emission from TW Hya (Qi et al. 2008; Figure 2).]]
  9 KB (1,372 words) - 22:05, 9 January 2017
• N891 simdata (CASA 3.4)
  * '''To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].''' ...using the Rayleigh-Jeans law: Jy/Sr = 2x10²³ k T / &lambda;² = 4x10⁸T at 110GHz.''
  5 KB (809 words) - 11:25, 24 October 2012
• PlotBasics
  2. You can use the matplotlib.pyplot environment, with plotting commands and axes2_range[2:4] = 3.26*axes1_range[2:4]/1000.0 # set second y-axis to Gly
  17 KB (2,938 words) - 18:54, 17 November 2011
• Karl G. Jansky VLA Tutorials-archived
  ...casa.shtml Previous CASA Versions] on the [https://casa.nrao.edu CASA home page]. === CASA 6.5.2 versions ===
  21 KB (2,724 words) - 12:03, 1 March 2024
• AngularSeparationOfFields
  This page documents the '''angularSeparationOfFields''' function of Python module [[A CASA <4>: au.angularSeparationOfFields('uid___A002_X49a70a_X4d8.ms', fields=[2])
  3 KB (301 words) - 01:03, 27 January 2013
• Lstrange
  This page documents the lstrange function of Python module [[Analysis Utilities|analy Found scans = [ 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27
  2 KB (265 words) - 11:50, 1 March 2012
• PPdisk simdata (CASA 3.2)
  ''A new version of this page exists for CASA 3.3: [[PPdisk simdata (CASA 3.3)]].'' *Simdata version for CASA 3.2
  4 KB (476 words) - 16:27, 3 November 2011
• AntennaeBand7
  ...respond to the CO(1-0) intensity map in Wilson et al. (2000; see also Fig. 2). (Credit: NASA, ESA, and the Hubble Heritage Team STScI/AURA-ESA/Hubble Co [[File:Wilson00-antennaeco1-0.jpg|300px|thumb|right|'''Fig. 2.''' Caltech millimeter array (OVRO) CO(1-0) integrated intensity map from W
  11 KB (1,652 words) - 04:27, 31 December 2023
• Planet
  This page documents the '''planet''' function of Python module [[Analysis Utilities|a 'directionRadians': [2.1579522305263157, 0.27351509191740353],
  8 KB (983 words) - 16:28, 6 September 2013
• Loading Data
  ...ther sign into your NRAO account (using the link at the top of the archive page) or obtain the Project Access Key from the [mailto:analysts@aoc.nrao.edu NR ...the [http://casa.nrao.edu/Memos/229.html MeasurementSet definition version 2.0].
  18 KB (2,494 words) - 10:53, 19 September 2019
• Baseband Stitching
  # [2,9]) 2 64 TOPO 4488 2000 128000 RR RL LR LL
  11 KB (1,530 words) - 21:09, 1 March 2012
• AntennaeBand7 for CASA 3.3
  ...respond to the CO(1-0) intensity map in Wilson et al. (2000; see also Fig. 2). (Credit: NASA, ESA, and the Hubble Heritage Team STScI/AURA-ESA/Hubble Co [[File:Wilson00-antennaeco1-0.jpg|200px|thumb|right|'''Fig. 2.''' Caltech millimeter array (OVRO) CO(1-0) integrated intensity map from W
  9 KB (1,443 words) - 12:08, 22 November 2011
• NGC3256Band3
  [[File:CO2-1_image_SMA.jpg|200px|thumb|right|SMA map of CO (2–1) emission in the center of NGC 3256 (Sakamoto, Ho & Peck, 2006)]] ...t extend up to 50 kpc. High-resolution observations of carbon-monoxide (CO 2-1) in NGC 3256 were made by Sakamoto et al. (2006) using the Submillimeter
  9 KB (1,395 words) - 09:09, 7 September 2015
• Baseband Stitching-CASA4.1
  # [2,9]) 2 64 TOPO 4488 2000 128000 RR RL LR LL
  11 KB (1,581 words) - 13:47, 1 May 2013
• CASA Contributed Script: vlacal-setjy
  This page is currently under development. MeasurementSet Name: vlacal_example.ms MS Version 2
  14 KB (1,935 words) - 23:52, 10 November 2021
• NGC3256Band3 for CASA 3.3
  [[File:CO2-1_image_SMA.jpg|200px|thumb|right|SMA map of CO (2–1) emission in the center of NGC 3256 (Sakamoto, Ho & Peck, 2006)]] ...t extend up to 50 kpc. High-resolution observations of carbon-monoxide (CO 2-1) in NGC 3256 were made by Sakamoto et al. (2006) using the Submillimeter
  8 KB (1,256 words) - 10:57, 26 April 2012
• BuildConfigurationFile
  This page documents the buildConfigurationFile function of Python module [[Analysis U CASA <2>: au.buildConfigurationFile('spw0_1.ms')
  6 KB (1,030 words) - 16:45, 24 March 2013
• NGC3256Band3 (Caltech)
  [[File:CO2-1_image_SMA.jpg|200px|thumb|right|SMA map of CO (2–1) emission in the center of NGC 3256 (Sakamoto, Ho & Peck, 2006)]] ...t extend up to 50 kpc. High-resolution observations of carbon-monoxide (CO 2-1) in NGC 3256 were made by Sakamoto et al. (2006) using the Submillimeter
  9 KB (1,372 words) - 01:46, 19 January 2012
• Imaging M99
  ...n angular size, which has been cleaned down to a threshold of 50mJy (about 2 sigma) and has been primary-beam corrected (see 'minpb' and 'pbcor'): clean(vis=msfile,imagename='clean_pb',spw='1~2',field='NGC4254',
  5 KB (806 words) - 13:38, 29 April 2010
• PythonDataAccess
  50:[1,2,3,5], b = 2
  5 KB (960 words) - 11:21, 2 November 2011
• Spectralindex
  This page documents the '''spectralindex''' function of the linfit class in the Pytho spw: the spws to use, e.g. ""=all, "1~3,5,6~8"=[1,2,3,5,6,7,8]
  8 KB (1,058 words) - 12:56, 8 August 2013
• Simulating Observations in CASA 3.4
  ...to simulate an observation in CASA. simobserve turns a model of the sky (2 to 4 dimensions including frequency and polarization) into the visibilities | rowspan=2 style="border-bottom:1px solid black;" | [[File:30Dor_ES.png|100px]]
  8 KB (1,207 words) - 13:02, 3 November 2015
• AntennaeBand7 3.4
  ...respond to the CO(1-0) intensity map in Wilson et al. (2000; see also Fig. 2). (Credit: NASA, ESA, and the Hubble Heritage Team STScI/AURA-ESA/Hubble Co [[File:Wilson00-antennaeco1-0.jpg|200px|thumb|right|'''Fig. 2.''' Caltech millimeter array (OVRO) CO(1-0) integrated intensity map from W
  10 KB (1,605 words) - 11:54, 30 May 2012
• PPdisk simdata (CASA 3.3)
  ''Old version: [[PPdisk simdata (CASA 3.2)]].'' To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].
  6 KB (798 words) - 11:17, 22 November 2011
• Simulating Observations in CASA 4.4
  ...<tt>simalma</tt> is to follow the tutorial linked near the bottom of this page. ...See [http://casaguides.nrao.edu/index.php?title=Convert_jpg_to_fits this page] for an example of using <tt>gimp</tt> to convert a JPG image to a FITS fil
  14 KB (2,193 words) - 10:17, 20 November 2015
• EVLA high frequency spectral line tutorial - IRC+10216 - calibration
  '''This page is under development''' 2 D J0954+1743 09:54:56.82363 +17.43.31.2224 J2000 2 32726
  13 KB (1,838 words) - 17:57, 6 January 2012
• Simulating Observations in CASA 4.2
  * '''This guide is applicable to CASA version 4.2. For older versions of CASA please see [[Simulating Observations in CASA 4 ...<tt>simalma</tt> is to follow the tutorial linked near the bottom of this page.
  14 KB (2,192 words) - 12:59, 3 November 2015
• ALMA2014 LBC SVDATA
  ...ortals, while the imaging scripts and salient details are provided on this page (the final target 3C138, will be released separately with other SV polariza ...ascience.nrao.edu/alma-data/science-verification Science Verification data page]:
  16 KB (2,452 words) - 10:11, 8 May 2018
• Simulating Observations in CASA 4.3
  ...For older versions of CASA please see [[Simulating Observations in CASA 4.2]]. --> ...<tt>simalma</tt> is to follow the tutorial linked near the bottom of this page.
  14 KB (2,261 words) - 09:02, 14 December 2018
• Simulating Observations in CASA 4.1
  ...nfiguration, and date for the simulated observation. The [[Antenna List]] page describes how to specify the telescope, including new telescopes, in more d | rowspan=2 style="border-bottom:1px solid black;" | [[File:30Dor_ES.png|100px]]
  12 KB (1,863 words) - 13:00, 3 November 2015
• Imaging Prep CASA 6.1.1
  Commands for this page can be found in scriptForImagingPrep_template.py available on [https://gith [[File:Weblog_Home.png|thumb|Figure 1: The Observation Overview page is opened with index.html.]]
  22 KB (2,892 words) - 16:28, 28 February 2024
• ALMA apply uvcont table
  ...NS OF THE C4 GUIDE; NEED TO UPDATE LINKS TO NEW C4 PAGE AND/OR LINK THE C5 PAGE INVOLVING REVISING THE RANGES'''). If you wish to revise the continuum sub This is a draft page describing how PI's can make use of the UVCONT table that is delivered with
  8 KB (1,144 words) - 11:09, 29 September 2017
• Simulation Guide for New Users (CASA 4.0)
  * '''To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].''' ...[http://casaguides.nrao.edu/index.php?title=Sim_Inputs Simulation Inputs] page for other sample images.
  15 KB (2,449 words) - 15:03, 2 November 2012
• SearchFlux
  This page documents the '''searchFlux''' function of Python module [[Analysis Utiliti 2 | 5.630 +- .02 | 2014-04-11 | 91.46 GHz | 0.0 | J1924-2914 |
  4 KB (421 words) - 14:16, 18 April 2014
• Imaging Prep CASA 6.5.4
  Commands for this page can be found in scriptForImagingPrep_template.py available on [https://gith [[File:Weblog_Home.png|thumb|Figure 1: The Observation Overview page is opened with index.html.]]
  23 KB (2,951 words) - 13:49, 7 December 2023
• Simulation Guide for New Users (CASA 3.4)
  * '''To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].''' ...[http://casaguides.nrao.edu/index.php?title=Sim_Inputs Simulation Inputs] page.
  16 KB (2,534 words) - 09:56, 24 October 2012
• Simulation Guide for New Users (CASA 3.3)
  ...tructions for older versions of CASA see [[Simdata New Users Guide (CASA 3.2)]].'' To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].
  16 KB (2,658 words) - 11:14, 22 November 2011
• Simulation Guide for New Users (CASA 4.2)
  * '''This guide is applicable to CASA version 4.2. For older versions of CASA see [[Simulation Guide for New Users (CASA 4.1 * '''To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].'''
  15 KB (2,491 words) - 10:53, 25 October 2013
• Simulation Guide for New Users (CASA 4.1)
  * '''To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].''' ...[http://casaguides.nrao.edu/index.php?title=Sim_Inputs Simulation Inputs] page for other sample images.
  15 KB (2,486 words) - 12:08, 24 October 2013
• Calibrating M99
  ...the mosaicked source fields are assigned FldId 2 through 20 (that's field='2~20' in python), and an extra "test" calibrator was also observed (3C274) an ...ennas. In this case, the narrowband windows are assigned to SpwID of 1 and 2, and they each have 63 channels. The reference antenna is Antenna 9, which
  12 KB (1,968 words) - 13:26, 29 April 2010
• Simdata New Users Guide (CASA 3.2)
  ''A new version of this page exists for CASA 3.3: [[Simulation Guide for New Users (CASA 3.3)]].'' ...ng scripts from these tutorials]] to extract a casapy script from this web page.
  16 KB (2,523 words) - 15:47, 6 October 2011
• Create a Clean Mask from Continuum Image or Moment Cube
  ...icient and reproducible to create a CLEAN mask from the data itself. This page outlines how to do this for continuum data (from the dirty image) and for s 2. **Don't forget to select "ALL CHANNELS" before editing the CLEAN mask (if
  3 KB (544 words) - 11:41, 9 July 2015
• Plotconfig
  This page documents the '''plotconfig''' function of Python module [[Analysis Utiliti Example 2. Plot the antenna pad locations for the ALMA Cycle 0 compact configuration.
  4 KB (325 words) - 11:47, 3 July 2013
• IRAS16293Band9
  ...2008). The emission is integrated over the velocity channels from V_lsr=-7.2 to 3.3 km/s on the blueshifted side and from V_lsr=5.5 to 31.9 km/s on the ...as shown in Figure 1. The complete 7 pointing mosaic can be seen in Figure 2, superposed on archival SMA data for better visualization.
  12 KB (1,832 words) - 23:18, 30 January 2024
• Complex pointingtable
  To create a script of the Python code on this page see [[Extracting scripts from these tutorials]]. Also, we want to add a calibrator at 2:12:32.0 -30.10.04.0, observed every 10 minutes for 18 sec.
  6 KB (959 words) - 17:01, 10 November 2011
• Complex pointingtable (CASA 3.4)
  To create a script of the Python code on this page see [[Extracting scripts from these tutorials]]. Also, we want to add a calibrator at 2:12:32.0 -30.10.04.0, observed every 10 minutes for 18 sec.
  6 KB (950 words) - 09:32, 8 June 2012
• WorkshopSelfcal (Caltech)
  '''This page steps through self-calibration of ALMA Science Verification data.''' ...y by carrying out self-calibration on ALMA Science Verification data. This page describes the data and introduces the scripts to do so. It is not a full-fl
  10 KB (1,646 words) - 03:38, 18 January 2012
• WorkshopSelfcal
  '''This page steps through self-calibration of the Science Verification data.''' ...ation on ALMA Science Verification data to improve the image quality. This page describes the data and introduces the scripts. It is not a full-fledged CAS
  9 KB (1,578 words) - 10:49, 27 February 2013
• Simalma (CASA 4.2)
  ...t Array (ACA). To learn how to create a script of the Python code on this page see [[Extracting scripts from these tutorials]]. ...observe a larger area on the sky than the main array antennas, by about 1/2 of a primary beam. So, it is generally better to generate the total power
  10 KB (1,648 words) - 11:54, 25 October 2013
• WorkshopImaging
  ...LMA Science Verification data to explore CASA's imaging capabilities. This page describes the data and introduces the scripts. It is not a full-fledged CAS ...ution (they are "FDM" mode) and cover the 850 micron continuum, the CO J=3-2 line, and HCO+ J=4-3 line. There is a full CASA Guide describing the reduct
  21 KB (3,592 words) - 16:03, 26 February 2013
• Simulating Observations in CASA 4.0
  ....html <tt>simanalyze</tt>]. <tt>simobserve</tt> turns a model of the sky (2 to 4 dimensions including frequency and polarization) into the visibilities | rowspan=2 style="border-bottom:1px solid black;" | [[File:30Dor_ES.png|100px]]
  12 KB (1,773 words) - 13:00, 3 November 2015
• EVLA high frequency Spectral Line Tutorial - CDE
  2 D J0954+1743 09:54:56.82363 +17.43.31.2224 J2000 2 32726 Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
  13 KB (1,853 words) - 13:35, 9 January 2012
• Fit an arbitrary sky (image) model to an existing MS
  ...ugh for absolute goodness of fit please note the caveat at the end of this page!). They could also be the starting point for a more comprehensive and sophi ...u if you set <b>defaultaxes=False</b> with the appropriate sub-parameters; 2) the simutil() module will allow you to do it. We illustrate the second cas
  12 KB (2,073 words) - 10:46, 15 March 2022
• Simulation Guide for New Users (CASA 4.3)
  .... For older versions of CASA see [[Simulation Guide for New Users (CASA 4.2)]].''' * '''To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].'''
  15 KB (2,490 words) - 20:49, 24 March 2015
• Simulation Guide for New Users (CASA 4.4)
  * '''To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].''' ...[http://casaguides.nrao.edu/index.php?title=Sim_Inputs Simulation Inputs] page for other sample images.
  15 KB (2,490 words) - 18:24, 6 July 2015
• Simalma (CASA 4.1)
  ...t Array (ACA). To learn how to create a script of the Python code on this page see [[Extracting scripts from these tutorials]]. ...observe a larger area on the sky than the main array antennas, by about 1/2 of a primary beam. So, it is generally better to generate the total power
  9 KB (1,510 words) - 18:06, 23 October 2013
• Notes on EVLA OSRO continuum data sets
  minpb = 0.2 # Minimum PB level to use ...ows. In this case, imaging can be greatly improved by setting '''nterms='''2 (or perhaps even higher), so that clean will fit a line to each source's sp
  5 KB (667 words) - 14:05, 25 March 2010
• Simdata New Users Guide 3.1
  ...asaguides.nrao.edu/index.php?title=Sim_Inputs Simulation Inputs CASA Guide page]. ...to rescale the pixels to shrink the image by roughly a factor of 15 (from 2.3" to 0.15" pixels) so that the model is approximately 40" on a side. This
  14 KB (2,317 words) - 18:01, 17 May 2011
• Simalma (CASA 4) original
  To create a script of the Python code on this page see [[Extracting scripts from these tutorials]]. ...ic. (For example it is generally recommended to observe a larger area by 1/2 primary beam in total power mode to combine with a 12 m ALMA mosaic).
  8 KB (1,330 words) - 17:23, 21 March 2024
• ALMA SIS14 apcal
  2014-03-06 19:09:04 INFO listobs 07:44:45.2 - 07:47:01.2 7 1 Ceres 5060 [0] [6.05] [CALIBRATE_AMPLI#O ...-06 19:09:04 INFO listobs 07:52:42.0 - 07:53:47.6 10 2 J1037-295 2760 [0] [6.05] [CALIBRATE_PHASE#ON_SOURCE, CAL
  20 KB (3,099 words) - 00:21, 7 March 2014
• Simalma (CASA 4.4)
  ...t Array (ACA). To learn how to create a script of the Python code on this page see [[Extracting scripts from these tutorials]]. ...observe a larger area on the sky than the main array antennas, by about 1/2 of a primary beam. So, it is generally better to generate the total power
  10 KB (1,607 words) - 10:42, 7 October 2015

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