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• 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

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