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• VLBI Tutorials
  ...[https://casaguides.nrao.edu/index.php/AIPS-Spectral_Lines_and_Astrometry Spectral Lines and Astrometry] ...//www.jb.man.ac.uk/DARA/unit4/Workshops/Spectral_line.html EVN HI Spectral Line]
  4 KB (593 words) - 18:09, 2 June 2023
• ALMAguides old
  ...at spectral line imaging in CASA]] This guide shows imaging of a spectral line.
  6 KB (859 words) - 16:29, 8 January 2018
• NGC3256 Band3 - Imaging (Caltech)
  [[Category:ALMA]][[Category:Imaging]][[Category:Spectral Line]] ...tech)]]''' CASA Guide will cover the imaging of the continuum and spectral line data. It begins where the '''[[NGC3256 Band3 - Calibration (Caltech)]]'''
  24 KB (3,568 words) - 21:20, 12 January 2012
• NGC3256 Band3 - Imaging for CASA 3.3
  [[Category:ALMA]][[Category:Imaging]][[Category:Spectral Line]] ...Band3]]''' CASA Guide will cover the imaging of the continuum and spectral line data. It begins where the '''[[NGC3256 Band3 - Calibration]]''' section le
  24 KB (3,580 words) - 05:18, 11 May 2012
• What's the difference between Antenna1 and Antenna2? Axis definitions in plotms
  ...r (analogous to what VLA users know as an IF). The characteristics of each spectral window are listed in {{listobs}}. * the rest frequency of the spectral line.
  5 KB (842 words) - 18:01, 7 June 2010
• ADMIT Products and Usage CASA 5.4.0
  ...tify spectral features, and create moment maps of each identified spectral line. ...s using the online version of Splatalogue rather than the internal one for line identification. These can be tuned via creating a file with your parameter
  15 KB (2,623 words) - 16:10, 28 February 2024
• NGC3256 Band3 Imaging for CASA 4.1
  [[Category:ALMA]][[Category:Imaging]][[Category:Spectral Line]] ...SA Guide for CASA 4.1 will cover the imaging of the continuum and spectral line data. It begins where the '''[[NGC3256 Band3 Calibration for CASA 4.1]]'''
  24 KB (3,681 words) - 09:10, 19 April 2013
• NGC3256 Band3 Imaging for CASA 3.4
  [[Category:ALMA]][[Category:Imaging]][[Category:Spectral Line]] ...SA Guide for CASA 3.4 will cover the imaging of the continuum and spectral line data. It begins where the '''[[NGC3256 Band3 Calibration for CASA 3.4]]'''
  24 KB (3,683 words) - 10:44, 1 June 2012
• NGC3256 Band3 Imaging for CASA 4.0
  [[Category:ALMA]][[Category:Imaging]][[Category:Spectral Line]] ...SA Guide for CASA 4.0 will cover the imaging of the continuum and spectral line data. It begins where the '''[[NGC3256 Band3 Calibration for CASA 4.0]]'''
  24 KB (3,681 words) - 13:14, 27 October 2012
• AntennaeBand7 North SS12
  [[Category:ALMA]][[Category:Calibration]][[Category:Spectral Line]] ...426 km/s); because the data are automatically Hanning smoothed, the actual spectral resolution is twice this. The TDM mode data were observed and used mainly f
  9 KB (1,381 words) - 10:20, 5 June 2012
• NGC3256 Band3 Imaging for CASA 4.2
  [[Category:ALMA]][[Category:Imaging]][[Category:Spectral Line]] ...SA Guide for CASA 4.2 will cover the imaging of the continuum and spectral line data. It begins where the '''[[NGC3256 Band3 Calibration for CASA 4.2]]'''
  24 KB (3,712 words) - 11:47, 29 November 2013
• HTT2
  * [[Selecting Spectral Windows and Channels]] *[[Applying EVLA on-line flags]] What do to if you need to re-apply (or apply) your online flags, wi
  3 KB (447 words) - 16:38, 30 October 2017
• Lstrange
  ...ent. It also lists the range of elevations on the target source, and a one-line summary that can be pasted into a table on the SCOPS wikipages. Note that t Ignoring spectral window [0, 25, 26, 27, 28, 29, 30, 31, 32, 33] because it is WVR related
  2 KB (265 words) - 11:50, 1 March 2012
• Obtaining Data: 3C 391 Example
  ...evel of time-average smearing. In this example, we opt not to perform any spectral or temporal averaging, and later show how this may be done after the fact b ...nations, particularly in compact configurations, one antenna may block the line of sight between another antenna and the source of interest. This effect i
  7 KB (1,170 words) - 16:58, 8 May 2016
• ADMIT Products and Usage CASA 6.5.4
  ...tify spectral features, and create moment maps of each identified spectral line. ...s using the online version of Splatalogue rather than the internal one for line identification. These can be tuned via creating a file with your parameter
  16 KB (2,805 words) - 16:18, 28 February 2024
• CASA Parallel Processing
  ...task level, <tt>pcont</tt> and <tt>pcube</tt> (for continuum and spectral line imaging, respectively). spw = '' # Select spectral window/channels
  11 KB (1,493 words) - 19:35, 8 May 2012
• Inspecting Data
  ...12 scans of ~1.5-minute duration each with 10s integrations. There are 15 spectral windows, the first half containing RR and second half with LL polarizations ...vation was done at night (the black disk represents the sun, below the red line, which is the horizon). The second panel shows the wind speed and directio
  10 KB (1,752 words) - 14:56, 9 August 2012
• OT tutorial SISS 2018
  ...define to propose for ALMA observations (spatial resolution, sensitivity, spectral setup), and to let you play with the ALMA OT so that you feel comfortable e * If it is an emission/absorption line experiment, the width of the frequency structure that you want to detect (i
  25 KB (4,152 words) - 11:36, 16 May 2018
• AntennaeBand7
  [[Category:ALMA]][[Category:Calibration]][[Category:Spectral Line]] ...duction and imaging of ALMA Science Verification data targeting the CO 3-2 line in the Antennae galaxy. These data were obtained using the ALMA Band 7 rece
  11 KB (1,652 words) - 04:27, 31 December 2023
• Data flagging with viewer
  ...s''' or '''channels''', the latter being particularly helpful for spectral-line experiments. ...ll probably also want to use the DVD-style control buttons to step through spectral channels. You can change which data dimension is affected by these control
  11 KB (1,676 words) - 10:56, 20 July 2017

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