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• Guide To Processing ALMA Data for Cycle 0
  # Image the H2D+ line structure (rest frequency 372.42138 GHz) # Image the N2H+ line structure (rest frequency 372.67249 GHz)
  46 KB (7,223 words) - 15:03, 7 September 2023
• Simulation Guide Component Lists (CASA 4.2)
  cs.setreferencevalue("230GHz",'spectral') cs.setincrement('1GHz','spectral')
  16 KB (2,530 words) - 11:24, 25 October 2013
• Simulation Guide Component Lists (CASA 4.1)
  cs.setreferencevalue("230GHz",'spectral') cs.setincrement('1GHz','spectral')
  16 KB (2,527 words) - 10:34, 10 May 2013
• Simulation Guide Component Lists (CASA 4.0)
  cs.setreferencevalue("230GHz",'spectral') cs.setincrement('1GHz','spectral')
  16 KB (2,531 words) - 16:15, 2 November 2012
• CASA Contributed Script: vlacal-setjy
  For this example, we would recommend the following line be included in publications using these data: * '''spw''': The CASA spectral window selection string to be processed. All SPWs need to be from the same
  14 KB (1,935 words) - 23:52, 10 November 2021
• Draft High Freq
  antennas and polarizations, robustness and line bandwidth to calculate Tell the on line system to apply those corrections to any number of
  25 KB (3,850 words) - 19:58, 17 August 2011
• SMA CO Line Data 3.1
  ...0. For an updated script that works with CASA 3.2.0, please go to [[SMA CO Line Data 3.2]].''' ...not use them for scientific purposes. This tutorial is based on the SMA CO Line Data script found in the [http://casa.nrao.edu/casascripts.shtml CASA Scrip
  41 KB (5,906 words) - 11:46, 18 May 2011
• M100 Band3 Combine 4.2.2
  == Split off CO spectral windows (SPWs) == ...e. Below are the first target scans of the 12m and 7m observations and the spectral window tables as generated by listobs. The six 7m data sets were taken with
  37 KB (5,642 words) - 19:30, 19 May 2015
• SMA CO Line Data 3.2
  ...not use them for scientific purposes. This tutorial is based on the SMA CO Line Data script found in the [http://casa.nrao.edu/casascripts.shtml CASA Scrip Spectral Windows:(24 unique spectral windows and 1 unique polarization setups)
  42 KB (6,040 words) - 13:25, 5 May 2011
• AntennaeBand7 Imaging 3.4
  ...<caption>'''Fig. 1.''' Southern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 50 to 100</caption>]] ...<caption>'''Fig. 2.''' Northern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 70 to 100</caption>]]
  44 KB (6,765 words) - 13:59, 11 October 2021
• CASA EVLA Scripts
  ...he MS (see example below) as well as estimate the zenith opacity for each spectral window. This script is only intended for use with the EVLA-- it contains h #edit the last line of the script, replacing MSname.ms with the name of your measurement set, a
  9 KB (1,452 words) - 11:40, 26 July 2013
• First Look at Self Calibration CASA 6
  ...window that we will image here as continuum also contains a N2H+ emission line. In this case, the N2H+ emission is faint enough that neglecting to flag the line channels before imaging makes no difference to the final continuum image.
  22 KB (3,254 words) - 12:48, 27 September 2023
• TWHydraBand7 SS12
  [[Category:ALMA]][[Category:Calibration]][[Category:Spectral Line]] ...libration, we inspect the data to understand the sequence of observations, spectral setup, what sources were observed, and the purpose of each observation. We
  64 KB (10,004 words) - 16:29, 31 May 2012
• DataWeightsAndCombination
  ...tasets, whereas Option 2 does not. However, see Caveat 1, for very complex line emission it may be difficult to get a good result. </span> ...tion, and it should always be run on the fully channelized data before any spectral averaging is applied.
  33 KB (5,060 words) - 17:27, 29 April 2024
• M100 Band3 SingleDish 4.2.2
  [[Category:ALMA]][[Category:Calibration]][[Category:Spectral Line]] Spectral Windows: (17 unique spectral windows and 2 unique polarization setups)
  39 KB (4,942 words) - 10:56, 4 August 2014
• AntennaeBand7 Imaging 4.0
  ...<caption>'''Fig. 1.''' Southern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 50 to 100</caption>]] ...<caption>'''Fig. 2.''' Northern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 70 to 100</caption>]]
  44 KB (6,844 words) - 15:05, 5 October 2021
• AntennaeBand7 Imaging 4.4
  ...<caption>'''Fig. 1.''' Southern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 50 to 100</caption>]] ...<caption>'''Fig. 2.''' Northern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 70 to 100</caption>]]
  44 KB (6,859 words) - 08:10, 5 October 2021
• AntennaeBand7 Imaging 4.1
  ...|<caption>'''Fig. 1.'''Southern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 50 to 100</caption>]] ...<caption>'''Fig. 2.''' Northern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 70 to 100</caption>]]
  44 KB (6,858 words) - 10:48, 5 October 2021
• AntennaeBand7 Imaging 4.2
  ...|<caption>'''Fig. 1.'''Southern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 50 to 100</caption>]] ...<caption>'''Fig. 2.''' Northern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 70 to 100</caption>]]
  44 KB (6,858 words) - 10:34, 5 October 2021
• AntennaeBand7 Imaging 4.5
  ...<caption>'''Fig. 1.''' Southern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 50 to 100</caption>]] ...<caption>'''Fig. 2.''' Northern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 70 to 100</caption>]]
  44 KB (6,883 words) - 07:26, 5 October 2021

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