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• EVLA high frequency Spectral Line tutorial - IRC+10216 part1
  [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] This tutorial describes the data reduction for two spectral lines observed toward the AGB star IRC+10216.
  53 KB (8,230 words) - 18:47, 17 May 2012
• VLA high frequency Spectral Line tutorial - IRC+10216
  79 bytes (11 words) - 10:04, 16 October 2020
• EVLA high frequency Spectral Line tutorial - IRC+10216 part2
  [[Image:irc10216_uvspec.png|thumb|UV-plot of the spectral line signal in both spw for IRC+10216.]] ...ls more precisely than is being done here due to time constraints, as weak line signal would not be obvious in this plot.
  28 KB (4,647 words) - 20:37, 29 February 2012
• EVLA high frequency spectral line tutorial - IRC+10216 - calibration
  ...ctral Line tutorial - IRC+10216 part1]] and [[EVLA high frequency Spectral Line tutorial - IRC+10216 part2]]. [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]]
  13 KB (1,838 words) - 17:57, 6 January 2012
• EVLA high frequency spectral line tutorial - IRC+10216 - imaging
  This tutorial picks up where [[ EVLA high frequency spectral line tutorial - IRC+10216 - calibration]] leaves off. [[Image:irc10216_uvspec.png|thumb|UV-plot of the spectral line signal in both spw for IRC+10216.]]
  3 KB (398 words) - 17:46, 6 January 2012
• EVLA high frequency Spectral Line tutorial - IRC+10216
  #REDIRECT [[EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.6]]
  76 bytes (10 words) - 16:22, 6 May 2016
• EVLA high frequency Spectral Line tutorial - IRC+10216 CASA3.4
  [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] This tutorial describes the data reduction for two spectral lines observed toward the AGB star IRC+10216.
  81 KB (12,845 words) - 16:03, 1 June 2012
• EVLA high frequency Spectral Line tutorial - IRC+10216-CASA3.4
  [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] This tutorial describes the data reduction for two spectral lines observed toward the AGB star IRC+10216.
  81 KB (12,853 words) - 22:34, 6 December 2012
• EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.0
  [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] This tutorial describes the data reduction for two spectral lines observed toward the AGB star IRC+10216.
  82 KB (13,029 words) - 16:14, 30 May 2013
• EVLA high frequency Spectral Line tutorial - IRC+10216-CAS4.0
  #REDIRECT [[EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.0]]
  76 bytes (10 words) - 19:31, 22 October 2012
• EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.1.0
  [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] This tutorial describes the data reduction for two spectral lines observed toward the AGB star IRC+10216.
  84 KB (13,072 words) - 21:45, 25 April 2013
• EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.3
  [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] This tutorial describes the data reduction for two spectral lines observed toward the AGB star IRC+10216.
  82 KB (12,857 words) - 13:35, 2 June 2015
• EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.4
  [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] This tutorial describes the data reduction for two spectral lines observed toward the AGB star IRC+10216.
  84 KB (13,101 words) - 13:57, 3 November 2015
• EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.6
  #REDIRECT [[VLA high frequency Spectral Line tutorial - IRC+10216-CASA4.6]]
  75 bytes (10 words) - 16:25, 6 May 2016
• EVLA high frequency Spectral Line tutorial - IRC+10216 part1 (Caltech)
  [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] This tutorial describes the data reduction for two spectral lines observed toward the AGB star IRC+10216.
  53 KB (8,284 words) - 01:44, 19 January 2012
• EVLA high frequency Spectral Line tutorial - IRC+10216 part2 (Caltech)
  This tutorial picks up where [[EVLA high frequency Spectral Line tutorial - IRC+10216 part1 (Caltech)]] leaves off. [[Image:irc10216_uvspec.png|thumb|UV-plot of the spectral line signal in both spw for IRC+10216.]]
  28 KB (4,570 words) - 17:09, 11 January 2012
• EVLA high frequency Spectral Line tutorial - IRC+10216 part1-CASA3.3
  [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] This tutorial describes the data reduction for two spectral lines observed toward the AGB star IRC+10216.
  52 KB (8,201 words) - 12:32, 9 April 2012
• EVLA high frequency Spectral Line tutorial - IRC+10216 part2-CASA3.3
  [[Image:irc10216_uvspec.png|thumb|UV-plot of the spectral line signal in both spw for IRC+10216.]] ...ls more precisely than is being done here due to time constraints, as weak line signal would not be obvious in this plot.
  28 KB (4,648 words) - 12:31, 9 April 2012
• VLA high frequency Spectral Line tutorial - IRC+10216-CASA4.6
  [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] This tutorial describes the data reduction for two spectral lines observed toward the Asymptotic Giant Branch (AGB) star IRC+10216.
  92 KB (14,496 words) - 16:50, 7 November 2016
• EVLA high frequency Spectral Line tutorial - IRC+10216 - CASA 4.2
  [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] This tutorial describes the data reduction for two spectral lines observed toward the AGB star IRC+10216.
  84 KB (13,082 words) - 17:15, 5 February 2014

Page text matches

• First Look at Line Imaging 4.4
  This lesson steps you through imaging of spectral lines. ...nuum self-cal solutions to our spectral line data to optimize our spectral line images.
  10 KB (1,580 words) - 11:13, 5 March 2018
• Spectral Viewer
  <big> '''A quick tutorial on how to use the Spectral Profile plotting tool, based on the CASA cookbook'''</big> == Opening the Spectral Profile plotting tool ==
  8 KB (1,247 words) - 01:21, 23 August 2012
• First Look at Image Analysis 4.4
  The first few tutorials provided us with a spectral line data cube and a continuum image. Next we'd like to line cube.
  5 KB (823 words) - 11:18, 5 March 2018
• List of All Tutorials
  ...VLA) '''Carbon Star <big>IRC+10216</big>: high frequency (36GHz), spectral line data reduction: ''' dataset size <font color=green>1.1GB</font> ** CASA 3.4: [[ EVLA high frequency Spectral Line tutorial - IRC+10216 CASA3.4| IRC+10216 Calibration+Imaging ]]
  8 KB (970 words) - 16:45, 10 June 2013
• WorkshopSelfcal
  ...e data. We will then see how to apply that self-calibration to improve the line images. ...interval and how you otherwise combine the data (averaging polarizations, spectral windows or channels, using a specific field in a mosaic). Try experimenting
  9 KB (1,578 words) - 10:49, 27 February 2013
• Karl G. Jansky VLA Tutorials
  ...CASA]. They offer examples for common general-use cases such as spectral line, continuum, linear polarization, and mosaicking. However, the results demo === High frequency (36GHz), spectral line data reduction: Carbon Star IRC+10216 ===
  13 KB (1,866 words) - 17:24, 25 March 2024
• First Look at Line Imaging CDE
  This lesson steps you through imaging of spectral lines. ...nuum self-cal solutions to our spectral line data to optimize our spectral line images.
  12 KB (1,869 words) - 15:05, 29 May 2019
• TWHydraBand7 for CASA 3.4 defunct
  [[Category:ALMA]][[Category:Calibration]][[Category:Spectral Line]] ...u/abs/2005ApJ...622.1171R Roberge et al. 2005]; Figure 7). The solid green line is the direction of maximum disk brightness at optical wavelengths.]]
  7 KB (1,192 words) - 12:47, 23 April 2012
• TWHydraBand7 For CASA 3.3
  [[Category:ALMA]][[Category:Calibration]][[Category:Spectral Line]] ...u/abs/2005ApJ...622.1171R Roberge et al. 2005]; Figure 7). The solid green line is the direction of maximum disk brightness at optical wavelengths.]]
  7 KB (1,195 words) - 12:49, 23 April 2012
• TWHydraBand7 For CASA 3.4
  [[Category:ALMA]][[Category:Calibration]][[Category:Spectral Line]] ...u/abs/2005ApJ...622.1171R Roberge et al. 2005]; Figure 7). The solid green line is the direction of maximum disk brightness at optical wavelengths.]]
  7 KB (1,210 words) - 13:09, 23 April 2012
• WorkshopSelfcal (Caltech)
  ...e data. We will then see how to apply that self-calibration to improve the line emission images. ...interval and how you otherwise combine the data (averaging polarizations, spectral windows or channels, using a specific field in a mosaic). Try experimenting
  10 KB (1,646 words) - 03:38, 18 January 2012
• First Look at Line Imaging CASA 5.7
  This lesson steps you through imaging of spectral lines. ...nuum self-cal solutions to our spectral line data to optimize our spectral line images.
  12 KB (1,972 words) - 17:16, 12 October 2023
• Notes on EVLA OSRO continuum data sets
  ..._the_Bandpasses | bandpass calibration]], just as you would for a spectral line data set; and spw = '' # Spectral windows e.g. '0~3', '' is all
  5 KB (667 words) - 14:05, 25 March 2010
• First Look at Line Imaging CASA 6
  This lesson steps you through imaging of spectral lines. ...nuum self-cal solutions to our spectral line data to optimize our spectral line images.
  13 KB (2,029 words) - 14:27, 6 April 2022
• First Look at Line Imaging CASA 6.4
  This lesson steps you through imaging of spectral lines. ...nuum self-cal solutions to our spectral line data to optimize our spectral line images.
  13 KB (2,029 words) - 16:28, 24 October 2022
• NGC3256Band3 for CASA 3.3
  [[Category:ALMA]][[Category:Calibration]][[Category:Spectral Line]] available basebands, which are associated with four different spectral windows: two
  8 KB (1,256 words) - 10:57, 26 April 2012
• Initial instructions for 2010
  ** Spectral Line: [[EVLA_Spectral_Line_Calibration_IRC%2B10216]] ** Spectral Line: [[EVLA_Spectral_Line_Calibration_IRC%2B10216]]
  4 KB (579 words) - 18:39, 10 June 2010
• TWHydraBand7 (Caltech)
  [[Category:ALMA]][[Category:Calibration]][[Category:Spectral Line]] ...u/abs/2005ApJ...622.1171R Roberge et al. 2005]; Figure 7). The solid green line is the direction of maximum disk brightness at optical wavelengths.]]
  8 KB (1,300 words) - 01:45, 19 January 2012

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