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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 = 2x10<sup>23</sup> k T / &lambda;<sup>2</sup>,
    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]]. ...;<sup>2</sup>, <!-- <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 = 2x10<sup>23</sup> k T / &lambda;<sup>2</sup> = 4x10<sup>8</sup>T 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
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  • 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
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  • 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
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  • 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).
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  • 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
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  • 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
  • Calibrating a Mosaicked Spectral Line Dataset
    '''Method 2''' ...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
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  • Importing and Calibrating a Mosaicked Spectral Line Dataset
    '''Method 2''' ...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
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  • Simalma (CASA 5.4)
    ...version 5.6.1. 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 (1,621 words) - 12:28, 19 February 2020
  • Simalma (CASA 4.3)
    ...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 (1,647 words) - 21:03, 24 March 2015
  • Einstein-Face (CASA 3.1)
    ..."truth" model is a familiar object or image. In this example (which is on page 13 of the [http://almatelescope.ca/ALMA-ESPrimer.pdf ALMA Early Science Pri '''Step 2:''' Convert your image to FITS
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  • ACA Simulation (CASA 4.2)
    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).
    9 KB (1,373 words) - 17:06, 22 October 2013
  • Simalma CASA 6.5.4
    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 (1,649 words) - 18:48, 26 March 2024
  • ACA Simulation (CASA 4.1)
    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).
    9 KB (1,374 words) - 16:50, 1 July 2013
  • Simalma (CASA 6.4.1)
    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 (1,671 words) - 14:24, 2 November 2022
  • Self-Calibration Template CASA 6.1.1
    ...tion, we set spwmap=[0,0,0] to map spw=0 to spw=0, spw=1 to spw=0, and spw=2 to spw=0. #nterms=2,
    21 KB (3,082 words) - 16:54, 28 February 2024
  • ALMA Pipeline Known Issues
    2. The tclean parameter psfphasecenter is still not functioning ([https://ope 2. hif_selfcal will fail for multi-EB single field projects with virtual spws
    25 KB (3,867 words) - 15:19, 13 March 2024
  • Simalma (CASA 6.1.1)
    ...lease-notes-610 CASA Docs]). Those bug fixes are not available in CASA 6.1.2, 6.1.0, and earlier version, so please use CASA 6.1.1 for the simalma task To learn how to create a script of the Python code on this page see [[Extracting scripts from these tutorials]].
    11 KB (1,727 words) - 14:48, 8 March 2021
  • ADMIT Products and Usage CASA 5.4.0
    ...e for that task) and a one-line explanation of what that task does (Figure 2). ...of that ADMIT task, clicking on the task name hyperlinks to the ADMIT wiki page for that task.</caption>]]
    15 KB (2,623 words) - 16:10, 28 February 2024
  • M100 Band3
    M100 Introduction Page. ...Array (NMA), the central 1' was mapped by Sakamoto et al. (1995, 1999) at 2.5" resolution. Its nucleus has also been mapped in CO using the IRAM interf
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  • Self-Calibration Template CASA 6.5.4
    ...tion, we set spwmap=[0,0,0] to map spw=0 to spw=0, spw=1 to spw=0, and spw=2 to spw=0. #nterms=2,
    22 KB (3,210 words) - 16:35, 11 October 2023
  • Corrupt
    For even more detail than is contained in this wiki page, please read this [https://safe.nrao.edu/wiki/pub/ALMA/SimulatorCookbook/co * '''mode'''="screen": a 2-dimensional phase screen is generated with the same fBM mathematical model,
    9 KB (1,379 words) - 17:17, 7 November 2012
  • Simalma (CASA 5.1)
    ...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
    10 KB (1,599 words) - 14:51, 9 September 2020
  • Plotbandpass
    This page documents the plotbandpass function of Python module [[Analysis Utilities|a True: figfile.1.png, figfile.2.png, etc.
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  • Guide To Simulating ALMA Data
    | rowspan=2; stype="border-bottom:1px solid black;" | [[File:Points-panels-hf.png | 200 | rowspan=2; stype="border-bottom:1px solid black;" | [[File:Gaussians-panels-hf.png |
    11 KB (1,742 words) - 17:03, 22 March 2024
  • Simulation Guide Component Lists (CASA 4.2)
    ''This guide is applicable to CASA version 4.2.'' To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].
    16 KB (2,530 words) - 11:24, 25 October 2013
  • Simulation Guide Component Lists (CASA 4.1)
    To create a script of the Python code on this page see [[Extracting scripts from these tutorials]]. ...ons given on the [http://casa.nrao.edu/casa_obtaining.shtml Obtaining CASA page].
    16 KB (2,527 words) - 10:34, 10 May 2013
  • Simulation Guide Component Lists (CASA 4.0)
    To create a script of the Python code on this page see [[Extracting scripts from these tutorials]]. ...ons given on the [http://casa.nrao.edu/casa_obtaining.shtml Obtaining CASA page].
    16 KB (2,531 words) - 16:15, 2 November 2012
  • IRAS16293 Band9 - Imaging for CASA 3.4
    were changed to correct for a 1.2" position error in the phase calibrator (1625-254). Without ...o do this, see the CASA 3.3 version of the guide linked at the top of this page for alternative (but slow) plotting options. Analysis Utilities are updated
    28 KB (4,108 words) - 16:24, 9 October 2012
  • IRAS16293 Band9 - Imaging for CASA 4.0
    were changed to correct for a 1.2" position error in the phase calibrator (1625-254). Without ...o do this, see the CASA 3.3 version of the guide linked at the top of this page for alternative (but slow) plotting options. Analysis Utilities are updated
    29 KB (4,266 words) - 17:07, 20 November 2012
  • TWHydraBand7 Simplified
    2 none TW Hya 11:01:51.84498 -34.42.17.1609 J2000 2 175176 2 1 TOPO 356716.625 1796875 1796875 XX YY
    49 KB (7,548 words) - 15:38, 9 May 2012
  • ADMIT Products and Usage CASA 6.5.4
    ...e for that task) and a one-line explanation of what that task does (Figure 2). ...of that ADMIT task, clicking on the task name hyperlinks to the ADMIT wiki page for that task.</caption>]]
    16 KB (2,805 words) - 16:18, 28 February 2024
  • IRAS16293 Band9 - Imaging for CASA 4.2
    were changed to correct for a 1.2" position error in the phase calibrator (1625-254). Without ..._Band9_-_Calibration_for_CASA_4.2 IRAS16293_Band9_-_Calibration_for_CASA_4.2] . If you completed the calibration section, then you already have the fina
    29 KB (4,388 words) - 11:43, 12 November 2014
  • IRAS16293 Band9 - Imaging for CASA 4.1
    were changed to correct for a 1.2" position error in the phase calibrator (1625-254). Without ...o do this, see the CASA 3.3 version of the guide linked at the top of this page for alternative (but slow) plotting options. Analysis Utilities are updated
    30 KB (4,407 words) - 20:48, 10 December 2013
  • VLA CASA Pipeline-CASA5.1.2
    '''This guide is designed for CASA 5.1.2''' [https://casa.nrao.edu/Data/EVLA/Pipeline/CASA5.1.2/html/ Pipeline Weblog]
    52 KB (8,196 words) - 14:51, 13 February 2018
  • TWHydraBand7 Old for CASA 3.3
    Observed from 22-Apr-2011/03:30:39.7 to 22-Apr-2011/05:00:47.2 (UTC) 2 none TW Hya 11:01:51.8450 -34.42.17.1609 J2000 2
    52 KB (7,967 words) - 17:18, 16 December 2011
  • ACA Simulation (CASA 4.3)
    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).
    9 KB (1,373 words) - 15:58, 15 January 2015
  • ACA Simulation (CASA 4.4)
    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).
    9 KB (1,373 words) - 10:05, 7 October 2015
  • ACA Simulation (CASA 5.1)
    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).
    9 KB (1,381 words) - 15:06, 23 January 2018
  • M51 at z = 0.1 and z = 0.3 (CASA 3.2)
    ''A new version of this page exists for CASA 3.3: [[M51 at z = 0.1 and z = 0.3 (CASA 3.3)]].'' ...ng scripts from these tutorials]] to extract a casapy script from this web page. Also notice that there are global python variables (e.g. fluxScale) which
    18 KB (2,815 words) - 09:46, 24 October 2011
  • EVLA Spectral Line Calibration IRC+10216
    ...pects are described in [[Getting_Started_in_CASA]]. You should review this page if you are new to CASA. In brief you can run CASA interactively by looking ...ng the method described at the [[Extracting_scripts_from_these_tutorials]] page.
    45 KB (7,121 words) - 14:11, 21 May 2012
  • ACA Simulation (CASA 5.4)
    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).
    10 KB (1,418 words) - 12:29, 19 February 2020
  • TWHydraBand7 Updated for CASA 3.3
    Observed from 22-Apr-2011/03:30:39.7 to 22-Apr-2011/05:00:47.2 (UTC) 2 none TW Hya 11:01:51.8450 -34.42.17.1609 J2000 2
    57 KB (8,983 words) - 12:55, 31 May 2012
  • TWHydraBand7 Calibration (Caltech)
    Observed from 22-Apr-2011/03:30:39.7 to 22-Apr-2011/05:00:47.2 (UTC) 2 none TW Hya 11:01:51.8450 -34.42.17.1609 J2000 2
    57 KB (9,025 words) - 15:30, 25 January 2012
  • VLA CASA Pipeline-CASA4.7.2
    '''This guide is designed for CASA 4.7.2''' [https://casa.nrao.edu/Data/EVLA/Pipeline/CASA4.7.2/html/ Pipeline Weblog]
    50 KB (7,973 words) - 18:32, 2 February 2018
  • CARMA spectral line mosaic M99 3.1
    ...pects are described in [[Getting_Started_in_CASA]]. You should review this page if you are new to CASA. In brief you can run CASA interactively by looking ...ng the method described at the [[Extracting_scripts_from_these_tutorials]] page.
    37 KB (5,752 words) - 17:27, 26 May 2011
  • TWHydraBand7 Calibration for CASA 3.3
    Observed from 22-Apr-2011/03:30:39.7 to 22-Apr-2011/05:00:47.2 (UTC) 2 none TW Hya 11:01:51.8450 -34.42.17.1609 J2000 2
    60 KB (9,450 words) - 16:45, 23 April 2012
  • ATCA Continuum Polarization Tutorial NGC612-CASA4.7
    [http://simbad.u-strasbg.fr/simbad/sim-id?Ident=NGC612&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id NGC612]. It has been adapted from the ...data were taken with 2048 MHz of bandwidth in 1 MHz channels, centered at 2.1 GHz, and recorded all polarizations.
    29 KB (3,228 words) - 01:23, 1 September 2020
  • VLA CASA Pipeline-CASA5.4.1
    '''This guide is designed for CASA 5.4.1. It should also run in CASA 5.4.2 which is an SRDP pipeline release that contains additional bookkeeping item ...the landing page one can find the items '''Home''' (the index.html landing page), '''By Topic''' and '''By Task''' that provide navigation through the pip
    59 KB (9,223 words) - 19:22, 18 June 2019
  • EVLA Spectral Line Calibration IRC+10216 - workshop
    ...pects are described in [[Getting_Started_in_CASA]]. You should review this page if you are new to CASA. In brief you can run CASA interactively by looking ...ng the method described at the [[Extracting_scripts_from_these_tutorials]] page.
    49 KB (7,632 words) - 21:16, 29 August 2011
  • CARMA spectral line mosaic M99 3.2
    ...pects are described in [[Getting_Started_in_CASA]]. You should review this page if you are new to CASA. In brief you can run CASA interactively by looking ...ng the method described at the [[Extracting_scripts_from_these_tutorials]] page.
    39 KB (6,041 words) - 13:04, 5 July 2011
  • ALMA Imaging Pipeline Reprocessing Tool
    - scriptForReprocessing.py # the tool described on this page ...# Examples: ’9:2,11:4,13:2,15:8’, ’*:2’
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  • Image Line CASA 6.1.1
    ...'1:0~259,1:501~3839'. The fitspw parameter should be '0,1:0~259,1:501~3839,2'. If you haven't installed Analysis Utilities, see [https://casaguides.nrao fitspw = '2:0~1200;1500~3839,3:0~1200;1500~3839' # line free channels. Use au.invertCha
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  • Simalma (CASA 5.4) v2
    ...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
    12 KB (1,972 words) - 15:13, 16 May 2019
  • Simulation Guide Component Lists (CASA 4.3)
    To create a script of the Python code on this page see [[Extracting scripts from these tutorials]]. ...ons given on the [http://casa.nrao.edu/casa_obtaining.shtml Obtaining CASA page].
    16 KB (2,530 words) - 15:56, 15 January 2015
  • Simulation Guide Component Lists (CASA 4.4)
    To create a script of the Python code on this page see [[Extracting scripts from these tutorials]]. ...ons given on the [http://casa.nrao.edu/casa_obtaining.shtml Obtaining CASA page].
    16 KB (2,530 words) - 18:26, 6 July 2015
  • EVLA high frequency Spectral Line tutorial - IRC+10216 part1-CASA3.3
    ...equency_Spectral_Line_tutorial_-_IRC%2B10216_part2-CASA3.3 IRC+10216 Part 2: continuum subtraction, imaging, selfcal] ...pects are described in [[Getting_Started_in_CASA]]. You should review this page if you are new to CASA. In brief you can run CASA interactively by looking
    52 KB (8,201 words) - 12:32, 9 April 2012
  • EVLA high frequency Spectral Line tutorial - IRC+10216 part1
    ..._high_frequency_Spectral_Line_tutorial_-_IRC%2B10216_part2 IRC+10216 Part 2: continuum subtraction, imaging, selfcal] ...pects are described in [[Getting_Started_in_CASA]]. You should review this page if you are new to CASA. In brief you can run CASA interactively by looking
    53 KB (8,230 words) - 18:47, 17 May 2012
  • VLA CASA Pipeline-CASA6.1.2
    '''This guide is designed for CASA 6.1.2.''' [https://casa.nrao.edu/Data/EVLA/Pipeline/CASA6.1.2/html/ Pipeline Weblog]
    60 KB (9,408 words) - 18:19, 7 July 2021
  • VLA CASA Pipeline-CASA5.6.2
    '''This guide is designed for CASA 5.6.2.''' [https://casa.nrao.edu/Data/EVLA/Pipeline/CASA5.6.2/html/ Pipeline Weblog]
    60 KB (9,524 words) - 17:19, 26 November 2019
  • EVLA high frequency Spectral Line tutorial - IRC+10216 part2 (Caltech)
    ...l only see signal in such a plot if (1) the data are well calibrated, and (2) there is significant signal near the phase center of the observations, or ...t to see what the variation in rms noise is. You should get something like 2 mJy. Note that the rms is much worse in channels with strong emission becau
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  • EVLA high frequency Spectral Line tutorial - IRC+10216 part1 (Caltech)
    cd /scr[2]/casa/ ...pects are described in [[Getting_Started_in_CASA]]. You should review this page if you are new to CASA. In brief you can run CASA interactively by looking
    53 KB (8,284 words) - 01:44, 19 January 2012
  • VLA CASA Bandpass Slope-CASA5.5.0
    .../aoc/sciops/jott/casa/topicalguide/bandpass/new/G192-BP.ms MS Version 2 .../06:31:48.0 - 06:36:42.0 6 0 3C147 704865 [0,1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,3
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  • EVLA high frequency Spectral Line tutorial - IRC+10216 part2
    ...l only see signal in such a plot if (1) the data are well calibrated, and (2) there is significant signal near the phase center of the observations, or ...t to see what the variation in rms noise is. You should get something like 2 mJy. Note that the rms is much worse in channels with strong emission becau
    28 KB (4,647 words) - 20:37, 29 February 2012
  • EVLA high frequency Spectral Line tutorial - IRC+10216 part2-CASA3.3
    ...l only see signal in such a plot if (1) the data are well calibrated, and (2) there is significant signal near the phase center of the observations, or ...t to see what the variation in rms noise is. You should get something like 2 mJy. Note that the rms is much worse in channels with strong emission becau
    28 KB (4,648 words) - 12:31, 9 April 2012
  • VLA CASA Bandpass Slope-CASA5.7.0
    .../aoc/sciops/jott/casa/topicalguide/bandpass/new/G192-BP.ms MS Version 2 .../06:31:48.0 - 06:36:42.0 6 0 3C147 704865 [0,1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,3
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  • VLA CASA Bandpass Slope-CASA6.2.0
    <b>This CASA Guide is for CASA version 6.2.0</b> ...[https://casaguides.nrao.edu/index.php/VLA_Continuum_Tutorial_3C391-CASA6.2.0 VLA 3C391 Continuum Tutorial] before proceeding with this tutorial.
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  • VLA-S-CASA Pipeline-CASA6.2.1
    '''This guide is designed for CASA 6.2.1.''' ...with the pipeline are discussed on the [[Pipeline: Frequent VLA problems]] page, where signatures and treatment of problematic data are discussed.
    60 KB (9,393 words) - 19:00, 28 February 2022
  • VLA CASA Pipeline-CASA6.2.1
    '''This guide is designed for CASA 6.2.1.''' [https://casa.nrao.edu/Data/EVLA/Pipeline/CASA6.2.1/html/ Pipeline Weblog]
    62 KB (9,729 words) - 17:59, 1 October 2021
  • IRAS16293 Band9 - Imaging for CASA 4.4
    were changed to correct for a 1.2" position error in the phase calibrator (1625-254). Without ...o do this, see the CASA 3.3 version of the guide linked at the top of this page for alternative (but slow) plotting options. Analysis Utilities are updated
    29 KB (4,388 words) - 21:53, 6 July 2015
  • ACA Simulation CASA 6.5.4
    ...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). To create a script of the Python code on this page, see: [[Extracting scripts from these tutorials]]<br>
    11 KB (1,560 words) - 13:33, 27 March 2024
  • IRAS16293 Band9 - Imaging for CASA 4.3
    were changed to correct for a 1.2" position error in the phase calibrator (1625-254). Without ...o do this, see the CASA 3.3 version of the guide linked at the top of this page for alternative (but slow) plotting options. Analysis Utilities are updated
    30 KB (4,388 words) - 11:03, 21 February 2018
  • Simulation Guide Component Lists (CASA 5.1)
    To create a script of the Python code on this page see [[Extracting scripts from these tutorials]]. ...ions given on the [http://casa.nrao.edu/casa_obtaining.shtml CASA download page].
    15 KB (2,339 words) - 13:37, 14 March 2018
  • VLA-S-CASA Pipeline-CASA6.4.1
    ...with the pipeline are discussed on the [[Pipeline: Frequent VLA problems]] page, where signatures and treatment of problematic data are discussed. ...the landing page one can find the items '''Home''' (the index.html landing page), '''By Topic''' and '''By Task''' that provide navigation through the pip
    62 KB (9,694 words) - 13:46, 17 January 2023
  • Simulation Guide Component Lists (CASA 5.4)
    To create a script of the Python code on this page see [[Extracting scripts from these tutorials]]. ...ions given on the [http://casa.nrao.edu/casa_obtaining.shtml CASA download page].
    15 KB (2,354 words) - 14:33, 15 February 2023
  • Simulation Guide Component Lists (CASA 6.5.3)
    To create a script of the Python code on this page see [[Extracting scripts from these tutorials]]. ...ions given on the [http://casa.nrao.edu/casa_obtaining.shtml CASA download page].
    15 KB (2,372 words) - 16:51, 15 February 2023
  • Antennae Band7 - Imaging for CASA 3.3
    ...ennae mosaics shown on the [[AntennaeBand7#ALMA_Data_Overview | Overview]] page are well-suited to joint deconvolution. However, if you have a poorly-sampl ...thumb|right|'''Fig. 1.''' Southern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 50 to 100]]
    41 KB (6,416 words) - 16:05, 16 May 2012
  • ACA Simulation (CASA 4.0)
    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).
    9 KB (1,293 words) - 18:45, 28 November 2012
  • EVLA Spectral Line Imaging Analysis IRC+10216
    ...l only see signal in such a plot if (1) the data are well calibrated, and (2) there is significant signal near the phase center of the observations, or ...t to see what the variation in rms noise is. You should get something like 2 mJy. Note that the rms is much worse in channels with strong emission becau
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  • Corrupting Simulated Data (Simulator Tool)
    For even more detail than is contained in this wiki page, please read this [https://safe.nrao.edu/wiki/pub/ALMA/SimulatorCookbook/co * '''mode'''="screen": a 2-dimensional phase screen is generated with the same fBM mathematical model,
    9 KB (1,379 words) - 15:36, 23 January 2018
  • TWHydraBand7 Calibration 3.4
    ...o do this, see the CASA 3.3 version of the guide linked at the top of this page for alternative (but slow) plotting options. Analysis Utilities are updated 2 none TW Hya 11:01:51.84498 -34.42.17.1609 J2000 2 175176
    76 KB (11,820 words) - 10:34, 25 July 2012
  • IRAS16293 Band9 - Imaging for CASA 4.5
    were changed to correct for a 1.2" position error in the phase calibrator (1625-254). Without ...o do this, see the CASA 3.3 version of the guide linked at the top of this page for alternative (but slow) plotting options. Analysis Utilities are updated
    26 KB (3,752 words) - 09:31, 4 April 2017
  • M51 at z = 0.1 and z = 0.3 (CASA 3.3)
    ...3.3. For older versions of CASA, see [[M51 at z = 0.1 and z = 0.3 (CASA 3.2)]].'' ...ls]], to extract a casapy script from this web page. Also notice that this page uses global Python variables (e.g. fluxScale), not to be confused with task
    22 KB (3,487 words) - 11:15, 22 November 2011
  • Draft High Freq
    ...solution is required for your science at the desired observing frequency; (2) for resolved sources, how does the desired angular resolution compare to t calibrator with 10 sigma on a single baseline (2 antennas) in a single
    25 KB (3,850 words) - 19:58, 17 August 2011
  • M51 at z = 0.1 and z = 0.3 (CASA 4.0)
    * '''To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].''' * '''Notice that this page uses global Python variables (e.g. fluxScale), not to be confused with task
    22 KB (3,420 words) - 15:28, 26 October 2012
  • ACA Simulation (CASA 3.4)
    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 12m ALMA mosaic).
    9 KB (1,326 words) - 10:37, 8 June 2012
  • ACA Simulation (CASA 3.3)
    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 12m ALMA mosaic).
    9 KB (1,364 words) - 18:51, 26 March 2024
  • TWHydraBand7 Calibration 4.0
    ...o do this, see the CASA 3.3 version of the guide linked at the top of this page for alternative (but slow) plotting options. Analysis Utilities are updated 2 none TW Hya 11:01:51.84498 -34.42.17.1609 J2000 2 175176
    78 KB (12,045 words) - 16:58, 7 November 2012
  • Image Line CASA 6.5.4
    ...'1:0~259,1:501~3839'. The fitspw parameter should be '0,1:0~259,1:501~3839,2'. If you haven't installed Analysis Utilities, see [https://casaguides.nrao fitspw = '2:0~1200;1500~3839,3:0~1200;1500~3839' # line free channels. Use au.invertCha
    16 KB (2,499 words) - 15:03, 18 October 2023
  • Calibrating an EVLA OSRO HI data set
    ...e calibration of an HI dataset collected on the Leo Ring with WIDAR0. This page will be updated when "real" OSRO data become available, but the below steps ...ntSet Name: /export/home/rso-lchomiuk/test/Leo/leotest.ms MS Version 2
    51 KB (6,414 words) - 17:21, 4 May 2010
  • M51 at z = 0.1 and z = 0.3 (CASA 3.1)
    ...ng scripts from these tutorials]] to extract a casapy script from this web page. ...tch roughly the BIMA SONG observation, a 4 MHz channel width), a factor of 2.5 greater than the anticipated contribution of noise from the model. Added
    17 KB (2,562 words) - 19:00, 28 April 2011
  • TWHydraBand7 SS12
    2 none TW Hya 11:01:51.84498 -34.42.17.1609 J2000 2 175176 2 1 TOPO 356716.625 1796875 1796875 XX YY
    64 KB (10,004 words) - 16:29, 31 May 2012
  • VLA-S-CASA Pipeline-CASA6.5.4
    ...with the pipeline are discussed on the [[Pipeline: Frequent VLA problems]] page, where signatures and treatment of problematic data are discussed. ...the landing page one can find the items '''Home''' (the index.html landing page), '''By Topic''' and '''By Task''' that provide navigation through the pip
    69 KB (10,685 words) - 12:46, 22 December 2023
  • TWHydraBand7 Calibration 4.1
    2 none TW Hya 11:01:51.84498 -34.42.17.1609 J2000 2 175176 2 none TW Hya 11:01:51.84498 -34.42.17.1609 J2000 2 175176
    78 KB (12,026 words) - 21:09, 10 December 2013
  • JuergensSandbox
    ...d rest frequencies by <math> v = \frac{\nu_0^{2} - \nu^{2}}{\nu_0^{2}+\nu^{2}}</math>. This equation is a bit cumbersome to use; in astronomy two differ ...rvation on the [http://www.vla.nrao.edu/cgi-bin/schedules.cgi VLA Schedule Page].
    42 KB (6,842 words) - 10:09, 2 July 2012
  • Image Continuum CASA 6.1.1
    ...gTemplate#Prepare for Imaging | Prepare for Imaging ]] section on the main page of this guide for more information. [[File:Calibrated_final_Field0_Spw3.png|thumb|Figure 2: Plots showing each spectral window for TW Hydra with channel vs amplitude.
    31 KB (4,832 words) - 16:33, 28 February 2024
  • AntennaeBand7 North Imaging 3.4
    ...e mosaics shown on the [[AntennaeBand7_3.4#ALMA_Data_Overview | Overview]] page are well-suited to joint deconvolution. However, if you have a poorly-sampl ...00px|thumb|right|<caption>Northern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 70 to 100</caption>]]
    40 KB (6,363 words) - 12:47, 5 June 2012
  • Image Continuum CASA 6.5.4
    ...gTemplate#Prepare for Imaging | Prepare for Imaging ]] section on the main page of this guide for more information. [[File:Calibrated_final_Field0_Spw3.png|thumb|Figure 2: Plots showing each spectral window for TW Hydra with channel vs amplitude.
    32 KB (5,048 words) - 14:42, 18 October 2023
  • M100 Band3 Combine 4.2.2
    This page is currently under construction. .../19:38:05.8 - 19:50:22.8 11 1 M100 1500 [0,1,2,3] [6.05, 6.05, 6.05, 6.05] [CALIBRATE_WVR#ON_SOURCE,OBSERVE_TARGET#ON_SOU
    37 KB (5,642 words) - 19:30, 19 May 2015
  • TWHydraBand7 Calibration 4.2
    *'''This guide is designed for CASA 4.2. If you are using an older version of CASA please see [[TWHydraBand7_Calib ...TWHYA_BAND7_UnCalibratedMSAndTablesForReduction CANNOT be used with CASA 4.2, they should be discarded, or moved out of the working directory.'''
    79 KB (12,189 words) - 16:20, 23 May 2014
  • M100 Band3 SingleDish 5.1
    ...interferometric (12-m array and 7-m array) data is explained in a separate page, valid for CASA versions 4.3 and later [[M100_Band3_Combine_4.3]]. uid___A002_X85c183_X36f Observed from 2014-07-01T21:51:26.2 to 2014-07-01T22:40:28.4 (UTC) DA61, PM03, PM04
    39 KB (5,284 words) - 16:07, 19 August 2021
  • M100 Band3 SingleDish 5.7
    *'''This guide is written for CASA 5.7 and uses Python 2. The same functionality is implemented in Python 3 using CASA 6.1 at [[M100 ...interferometric (12-m array and 7-m array) data is explained in a separate page [[M100_Band3_Combine_5.7]].
    39 KB (5,356 words) - 14:36, 19 August 2021
  • M100 Band3 SingleDish 6.1
    ...ASA 6.1 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_S ...interferometric (12-m array and 7-m array) data is explained in a separate page, valid for CASA versions 6.1 and later [[M100_Band3_Combine_6.1]].
    40 KB (5,435 words) - 14:37, 19 August 2021
  • AIPS-Simple-Self-Cal
    ...w.physics.purdue.edu/astro/MOJAVE/sourcepages/0851+202.shtml MOJAVE source page] ...w.physics.purdue.edu/astro/MOJAVE/sourcepages/1828+487.shtml MOJAVE source page]
    49 KB (7,800 words) - 17:42, 29 March 2022
  • M100 Band3 SingleDish 6.2
    *'''This guide is written for CASA 6.2 and uses Python 3''' ...processes described below WILL NOT OPERATE in CASA versions earlier than 6.2.0'''
    40 KB (5,491 words) - 11:39, 7 April 2022
  • EVLA spectral line IRC10216
    2 D J0954+1743 09:54:56.8236 +17.43.31.2224 J2000 2 65326 Spectral Windows: (2 unique spectral windows and 1 unique polarization setups)
    44 KB (6,777 words) - 12:19, 19 May 2010
  • M100 Band3 SingleDish 6.4
    ...interferometric (12-m array and 7-m array) data is explained in a separate page, valid for CASA versions 6.4 and later [[M100_Band3_Combine_6.4]]. uid___A002_X85c183_X36f Observed from 2014-07-01T21:51:26.2 to 2014-07-01T22:40:28.4 (UTC) DA61, PM03, PM04
    40 KB (5,491 words) - 11:06, 12 October 2023
  • M100 Band3 SingleDish 6.5.4
    ...interferometric (12-m array and 7-m array) data is explained in a separate page, valid for CASA versions 6.4 and later [[M100_Band3_Combine_6.4]]. uid___A002_X85c183_X36f Observed from 2014-07-01T21:51:26.2 to 2014-07-01T22:40:28.4 (UTC) DA61, PM03, PM04
    40 KB (5,472 words) - 16:52, 2 February 2024
  • ACA Simulation (CASA 5.4) v2
    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).
    13 KB (1,911 words) - 12:07, 8 May 2019
  • VLA CASA Bandpass Slope-CASA5.4.0
    .../aoc/sciops/jott/casa/topicalguide/bandpass/new/G192-BP.ms MS Version 2 .../06:31:48.0 - 06:36:42.0 6 0 3C147 704865 [0,1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,3
    27 KB (3,654 words) - 14:39, 6 November 2018
  • M100 Band3 SingleDish 4.5
    ...interferometric (12-m array and 7-m array) data is explained in a separate page, valid for both CASA versions 4.3 and 4.5 [[M100_Band3_Combine_4.3]]. uid___A002_X85c183_X36f Observed from 2014-07-01T21:51:26.2 to 2014-07-01T22:40:28.4 (UTC) DA61, PM03, PM04
    39 KB (5,283 words) - 01:21, 23 August 2017
  • M100 Band3 SingleDish 4.2.2
    This page is currently under construction. ....3 - 02:22:42.8 1 0 M100 900 0.00 [0, 1, 2, 3, 4, 5, 6, 7, 8] [1.15, 0.48, 0.48, 0.48, 0.48, 0.48, 0.48, 0.48, 0.48]
    39 KB (4,942 words) - 10:56, 4 August 2014
  • EVLA Wide-Band Wide-Field Imaging: G55.7 3.4-CASA3.3
    ...ng observation includes all available 1 GHz of bandwidth in L-band, from 1-2 GHz in frequency. ...before, some helpful tips are available on the [[Getting Started in CASA]] page.
    71 KB (9,680 words) - 12:37, 9 April 2012
  • AntennaeBand7 Imaging 3.4
    ...ennae mosaics shown on the [[AntennaeBand7#ALMA_Data_Overview | Overview]] page are well-suited to joint deconvolution. However, if you have a poorly-sampl ...ht|<caption>'''Fig. 1.''' Southern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 50 to 100</caption>]]
    44 KB (6,765 words) - 13:59, 11 October 2021
  • M51 at z = 0.1 and z = 0.3 (CASA 3.4)
    * '''To create a script of the Python code on this page see [[Extracting scripts from these tutorials]].''' * '''Notice that this page uses global Python variables (e.g. fluxScale), not to be confused with task
    22 KB (3,420 words) - 17:04, 1 September 2017
  • EVLA Wide-Band Wide-Field Imaging: G55.7 3.4 (Caltech)
    ...ng observation includes all available 1 GHz of bandwidth in L-band, from 1-2 GHz in frequency. cd /scr[2]/casa/
    72 KB (9,756 words) - 01:45, 19 January 2012
  • EVLA Wide-Band Wide-Field Imaging: G55.7 3.4-CASA4.0
    ...ng observation includes all available 1 GHz of bandwidth in L-band, from 1-2 GHz in frequency. ...before, some helpful tips are available on the [[Getting Started in CASA]] page.
    76 KB (10,592 words) - 15:24, 11 December 2012
  • AntennaeBand7 Imaging 4.0
    ...ennae mosaics shown on the [[AntennaeBand7#ALMA_Data_Overview | Overview]] page are well-suited to joint deconvolution. However, if you have a poorly-sampl ...ht|<caption>'''Fig. 1.''' Southern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 50 to 100</caption>]]
    44 KB (6,844 words) - 15:05, 5 October 2021
  • AntennaeBand7 Imaging 4.4
    ...ennae mosaics shown on the [[AntennaeBand7#ALMA_Data_Overview | Overview]] page are well-suited to joint deconvolution. However, if you have a poorly-sampl ...ht|<caption>'''Fig. 1.''' Southern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 50 to 100</caption>]]
    44 KB (6,859 words) - 08:10, 5 October 2021
  • AntennaeBand7 Imaging 4.1
    ...ennae mosaics shown on the [[AntennaeBand7#ALMA_Data_Overview | Overview]] page are well-suited to joint deconvolution. However, if you have a poorly-sampl ...ght|<caption>'''Fig. 1.'''Southern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 50 to 100</caption>]]
    44 KB (6,858 words) - 10:48, 5 October 2021
  • AntennaeBand7 Imaging 4.2
    * '''This guide is designed for CASA 4.2.0. If you are using an older version of CASA please see [[AntennaeBand7_Im * '''This tutorial picks up where [[AntennaeBand7_Calibration_4.2]] leaves off: with fully calibrated, split science target measurement sets.
    44 KB (6,858 words) - 10:34, 5 October 2021
  • AntennaeBand7 Imaging 4.5
    ...ennae mosaics shown on the [[AntennaeBand7#ALMA_Data_Overview | Overview]] page are well-suited to joint deconvolution. However, if you have a poorly-sampl ...ht|<caption>'''Fig. 1.''' Southern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 50 to 100</caption>]]
    44 KB (6,883 words) - 07:26, 5 October 2021
  • Sunspot Band6 Calibration for CASA 5.1
    ...ts and software of the package can be obtained from the Analysis Utilities page[https://casaguides.nrao.edu/index.php/Analysis_Utilities]. .../19:15:42.3 - 19:16:47.5 1 0 Sun 236530 [0,1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24] [0.016, 0.016,
    40 KB (4,408 words) - 16:31, 19 August 2021
  • EVLA Wide-Band Wide-Field Imaging: G55.7 3.4-CASA4.1
    ...ng observation includes all available 1 GHz of bandwidth in L-band, from 1-2 GHz in frequency. ...before, some helpful tips are available on the [[Getting Started in CASA]] page.
    77 KB (10,632 words) - 16:09, 2 May 2013
  • EVLA Wide-Band Wide-Field Imaging: G55.7 - CASA4.1
    ...ng observation includes all available 1 GHz of bandwidth in L-band, from 1-2 GHz in frequency. ...before, some helpful tips are available on the [[Getting Started in CASA]] page.
    77 KB (10,632 words) - 19:57, 4 February 2014
  • AntennaeBand7 Imaging 4.3
    ...ou are using an older version of CASA please see [[AntennaeBand7_Imaging_4.2]]. ...ennae mosaics shown on the [[AntennaeBand7#ALMA_Data_Overview | Overview]] page are well-suited to joint deconvolution. However, if you have a poorly-sampl
    44 KB (6,883 words) - 09:40, 5 October 2021
  • IRAS16293 Band9 - Imaging for CASA 5.1
    were changed to correct for a 1.2" position error in the phase calibrator (1625-254). Without ...o do this, see the CASA 3.3 version of the guide linked at the top of this page for alternative (but slow) plotting options. Analysis Utilities are updated
    36 KB (5,365 words) - 10:23, 28 September 2018
  • VLA CASA Flagging-CASA4.6.0
    ...r long session includes all available 1 GHz of bandwidth in L-band, from 1-2 GHz in frequency. ...DM-BDF dataset (all files)''' as the data download option on the following page. Be aware that the full dataset is 170GB!
    68 KB (9,089 words) - 18:34, 18 October 2016
  • VLA CASA Flagging-CASA4.5.2
    * '''This CASA guide is designed for CASA 4.5.2''' ...r long session includes all available 1 GHz of bandwidth in L-band, from 1-2 GHz in frequency.
    68 KB (9,104 words) - 18:34, 18 October 2016
  • Sunspot Band6 Calibration for CASA 4.7
    ...ts and software of the package can be obtained from the Analysis Utilities page[https://casaguides.nrao.edu/index.php/Analysis_Utilities]. .../19:15:42.3 - 19:16:47.5 1 0 Sun 236530 [0,1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24] [0.016, 0.016,
    41 KB (4,534 words) - 08:50, 11 January 2018
  • ATCA CABB Continuum Tutorial
    === (This Page is Currently Under Development) === ...at short scans of field 1 bracket longer scans of field 2051-377 (field ID 2), which is our science target.
    31 KB (4,564 words) - 02:04, 2 June 2015
  • AntennaeBand7 Imaging 6.5.4
    ...ennae mosaics shown on the [[AntennaeBand7#ALMA_Data_Overview | Overview]] page are well-suited to joint deconvolution. However, if you have a poorly-sampl ...ht|<caption>'''Fig. 1.''' Northern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 70 to 100</caption>]]
    51 KB (7,819 words) - 15:29, 29 February 2024
  • VLA CASA Pipeline-CASA4.7.0
    • CASA 4.5.2 currently being validated (you are helping with this!) ...ral use (see [https://casa.nrao.edu/casa_obtaining.shtml the CASA download page] for all pipeline versions). At NRAO, we will always execute the standard p
    83 KB (12,631 words) - 16:13, 10 October 2016
  • VLA CASA Pipeline-CASA4.5.3
    • CASA 4.5.2 currently being validated (you are helping with this!) ...ral use (see [https://casa.nrao.edu/casa_obtaining.shtml the CASA download page] for all pipeline versions). At NRAO, we will always execute the standard p
    84 KB (12,632 words) - 17:59, 29 March 2017
  • EVLA Wide-Band Wide-Field Imaging: G55.7 - CASA4.2
    * '''This CASA Guide is designed for CASA v4.2. If you are using an older version of CASA please see [[EVLA Wide-Band Wid [[EVLA Wide-Band Wide-Field Imaging: G55.7 - CASA4.2]]
    80 KB (11,156 words) - 17:30, 9 May 2014
  • VLA CASA Flagging-CASA4.7.0
    ...session includes all available 1 GHz of bandwidth in L-band, from 1&ndash;2 GHz in frequency. ...DM-BDF dataset (all files)''' as the data download option on the following page. Be aware that the full dataset is 170GB!
    69 KB (9,365 words) - 15:46, 19 July 2017
  • VLA CASA Flagging-CASA5.0.0
    ...session includes all available 1 GHz of bandwidth in L-band, from 1&ndash;2 GHz in frequency. ...DM-BDF dataset (all files)''' as the data download option on the following page. Be aware that the full dataset is 170GB!
    73 KB (9,761 words) - 12:19, 1 August 2017
  • VLA CASA Pipeline-full-CASA4.7.2
    '''This guide is designed for CASA 4.7.2''' ...ral use (see [https://casa.nrao.edu/casa_obtaining.shtml the CASA download page] for all pipeline versions). At NRAO, we will always execute the standard p
    85 KB (13,006 words) - 18:57, 19 May 2017
  • SMA CO Line Data 3.1
    [[File:g19.3CO.png|thumb| Integrated intensity SMA 12CO 2-1 map of G19.3+0.07 overlaid on a Spitzer image]] ...dated script that works with CASA 3.2.0, please go to [[SMA CO Line Data 3.2]].'''
    41 KB (5,906 words) - 11:46, 18 May 2011
  • TWHydraBand7 Calibration 4.4
    2 none TW Hya 11:01:51.84498 -34.42.17.1609 J2000 2 175176 2 none TW Hya 11:01:51.84498 -34.42.17.1609 J2000 2 175176
    79 KB (12,190 words) - 21:32, 6 July 2015
  • EVLA Wide-Band Wide-Field Imaging: G55.7 3.4-CASA3.4
    ...ng observation includes all available 1 GHz of bandwidth in L-band, from 1-2 GHz in frequency. ...before, some helpful tips are available on the [[Getting Started in CASA]] page.
    77 KB (10,677 words) - 15:29, 14 June 2012
  • EVLA Wide-Band Wide-Field Imaging: G55.7 3.4-CASA3.4-updated
    ...ng observation includes all available 1 GHz of bandwidth in L-band, from 1-2 GHz in frequency. ...before, some helpful tips are available on the [[Getting Started in CASA]] page.
    77 KB (10,677 words) - 13:28, 14 June 2012
  • TWHydraBand7 Calibration 4.3
    ...are using an older version of CASA please see [[TWHydraBand7_Calibration_4.2]]. 2 none TW Hya 11:01:51.84498 -34.42.17.1609 J2000 2 175176
    78 KB (11,957 words) - 16:55, 19 August 2021
  • OT tutorial SISS 2018
    2” is ~ 150 pc at the distance of M100. This doesn’t quite resolve indivi ...For a CO-to-H<sub>2</sub> conversion factor of ~2x10<sup>20</sup> cm<sup>-2</sup> (K km/s)<sup>-1</sup> and assuming a CO line width of 10 km/s, a 1&si
    25 KB (4,152 words) - 11:36, 16 May 2018
  • NGC3256 Band3 - Calibration for CASA 3.3
    2 none NGC3256 10:27:51.6000 -43.54.18.0000 J2000 2 151249 Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    58 KB (8,691 words) - 11:04, 23 November 2011
  • SMA CO Line Data 3.2
    [[File:g19.3CO.png|thumb| Integrated intensity SMA 12CO 2-1 map of G19.3+0.07 overlaid on a Spitzer image]] ...ound in the [http://casa.nrao.edu/casascripts.shtml CASA Scripts and Data] page.
    42 KB (6,040 words) - 13:25, 5 May 2011
  • VLA CASA Bandpass Slope-CASA4.5.2
    <b>This CASA Guide is for CASA version 4.5.2</b> .../aoc/sciops/jott/casa/topicalguide/bandpass/new/G192-BP.ms MS Version 2
    26 KB (3,524 words) - 10:41, 14 June 2016
  • TWHydraBand7 Calibration 4.5
    *'''This guide is designed for CASA 4.5.2 If you are using an older version of CASA please see [[TWHydraBand7_Calibr This guide has been written for CASA release 4.5.2. Please confirm your version before proceeding.
    81 KB (12,419 words) - 09:36, 10 April 2017
  • AntennaeBand7 Imaging 5.1
    ...ennae mosaics shown on the [[AntennaeBand7#ALMA_Data_Overview | Overview]] page are well-suited to joint deconvolution. However, if you have a poorly-sampl ...ht|<caption>'''Fig. 1.''' Southern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 50 to 100</caption>]]
    47 KB (7,341 words) - 16:35, 20 August 2021
  • VLA CASA Bandpass Slope-CASA4.7.0
    .../aoc/sciops/jott/casa/topicalguide/bandpass/new/G192-BP.ms MS Version 2 .../06:31:48.0 - 06:36:42.0 6 0 3C147 704865 [0,1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,3
    26 KB (3,524 words) - 13:14, 20 April 2017
  • VLA CASA Bandpass Slope-CASA4.6.0
    .../aoc/sciops/jott/casa/topicalguide/bandpass/new/G192-BP.ms MS Version 2 .../06:31:48.0 - 06:36:42.0 6 0 3C147 704865 [0,1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,3
    26 KB (3,524 words) - 11:47, 18 November 2016
  • NGC3256 Band3 - Calibration (Caltech)
    2 none NGC3256 10:27:51.6000 -43.54.18.0000 J2000 2 151249 Spectral Windows: (9 unique spectral windows and 2 unique polarization setups)
    58 KB (8,728 words) - 17:14, 25 January 2012
  • AntennaeBand7 Imaging 5.7
    *'''This guide is written for CASA 5.7 and uses Python 2. The same functionality is implemented in Python 3 using CASA 6.1 at [[Ante ...ennae mosaics shown on the [[AntennaeBand7#ALMA_Data_Overview | Overview]] page are well-suited to joint deconvolution. However, if you have a poorly-sampl
    49 KB (7,485 words) - 15:44, 20 August 2021
  • AntennaeBand7 Imaging 6.1
    ...ASA 6.1 and uses Python 3. The same functionality is implemented in Python 2 using CASA 5.7 at [[AntennaeBand7 Imaging 5.7]]''' ...ennae mosaics shown on the [[AntennaeBand7#ALMA_Data_Overview | Overview]] page are well-suited to joint deconvolution. However, if you have a poorly-sampl
    49 KB (7,492 words) - 13:22, 13 October 2021
  • AntennaeBand7 Imaging 5.4
    ...ennae mosaics shown on the [[AntennaeBand7#ALMA_Data_Overview | Overview]] page are well-suited to joint deconvolution. However, if you have a poorly-sampl ...ht|<caption>'''Fig. 1.''' Southern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 50 to 100</caption>]]
    48 KB (7,478 words) - 15:24, 20 August 2021

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