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  • * EVLA Ka-Band (36 GHz/10 mm) Spectral Line Observations of the AGB Star ([http://simbad.u-strasbg.fr/simbad/sim-id?Ide ** Data Calibration: [[EVLA Spectral Line Calibration IRC+10216]]
    775 bytes (114 words) - 13:26, 5 October 2010
  • * EVLA Ka-Band (36 GHz/10 mm) Spectral Line Observations of the AGB Star ([http://simbad.u-strasbg.fr/simbad/sim-id?Ide ** Data Calibration: [[EVLA Spectral Line Calibration IRC+10216]]
    1 KB (164 words) - 17:01, 30 November 2017
  • #REDIRECT [[EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.0]]
    76 bytes (10 words) - 19:31, 22 October 2012
  • #REDIRECT [[VLA high frequency Spectral Line tutorial - IRC+10216-CASA4.6]]
    75 bytes (10 words) - 16:25, 6 May 2016
  • #REDIRECT [[EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.6]]
    76 bytes (10 words) - 16:22, 6 May 2016
  • #REDIRECT [[VLA high frequency Spectral Line tutorial - IRC+10216-CASA4.7]]
    75 bytes (10 words) - 20:00, 17 November 2016
  • #REDIRECT [[MG0414+0534 P-band Spectral Line Tutorial - CASA 5.0.0]]
    68 bytes (8 words) - 13:32, 2 September 2017
  • #REDIRECT [[MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.4]]
    68 bytes (8 words) - 17:52, 29 February 2024
  • #REDIRECT [[MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.4]]
    68 bytes (8 words) - 17:52, 29 February 2024
  • #REDIRECT [[MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.2]]
    68 bytes (8 words) - 15:35, 13 February 2023
  • #REDIRECT [[HI 21cm (1.4 GHz) spectral line data reduction: LEDA 44055]]
    72 bytes (9 words) - 18:04, 4 February 2019
  • * Imaging from one spectral window to full dataset ...tral_Line_tutorial_-_IRC%2B10216_part1_%28Caltech%29 IRC+10216 -- Spectral line, Ka-band (36 GHz)]
    3 KB (383 words) - 14:22, 16 January 2012
  • #REDIRECT [[HI 21cm (1.4 GHz) spectral line data reduction: LEDA 44055-CASA6.5.2]]
    82 bytes (10 words) - 19:27, 16 November 2022
  • * Spectral Line calibration and imaging ...l illustrates calibration and imaging of a spectral cube spread across two spectral windows (VLA 4IF mode).
    585 bytes (71 words) - 19:16, 18 September 2018
  • 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
  • ...itions of the same line. This process increases the signal to noise of the line observations. It may not be suitable for all science cases. ...ctral window. The data were calibrated and split off so that each spectral line had its own visibility set.
    5 KB (757 words) - 22:04, 23 April 2012
  • ...534_P-band_Spectral_Line_Tutorial_-_CASA_6.5.4 MG0414+0534 P-band Spectral Line Tutorial (CASA 6.5.4)] ...534_P-band_Spectral_Line_Tutorial_-_CASA_6.5.2 MG0414+0534 P-band Spectral Line Tutorial (CASA 6.5.2)]
    21 KB (2,724 words) - 12:03, 1 March 2024
  • ...frequency Spectral Line tutorial - IRC+10216 CASA3.4 | IRC+10216 Spectral Line]] </big> </big> ** <big> <big> [[CARMA spectral line mosaic M99 3.2| M99 Spectral Line Mosaic]] </big> </big>
    6 KB (854 words) - 18:09, 14 November 2012
  • ...irty image) and for spectral line data (from the moment 0 map of the dirty line cube). First make a spectral line and/or continuum "dirty map" by calling CLEAN with niter=0. This is the sta
    3 KB (544 words) - 11:41, 9 July 2015
  • 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
  • <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
  • 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
  • ...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
  • ...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
  • ...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
  • 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
  • [[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
  • [[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
  • [[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
  • ...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
  • 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
  • ..._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
  • 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
  • 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
  • [[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
  • ** 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
  • [[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
  • 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 (1,997 words) - 16:21, 12 October 2023
  • [[Category:ALMA]][[Category:Calibration]][[Category:Spectral Line]] available basebands, which are associated with four different spectral windows: two
    9 KB (1,372 words) - 01:46, 19 January 2012
  • The first few tutorials provided us with a spectral line data cube and a continuum image. Next we'd like to ImageMetaData Spectral reference : LSRK (-> TOPO)
    9 KB (1,122 words) - 14:53, 29 May 2019
  • ...Imaging]]''' This page performs continuum subtraction and creates spectral line cubes using the MS created in [[Imaging_Prep | Prepare the data for imaging #'''[[Image Line CASA 6.1.1]]'''
    7 KB (1,132 words) - 16:55, 28 February 2024
  • The first few tutorials provided us with a spectral line data cube and a continuum image. Next we'd like to ImageMetaData Spectral reference : LSRK
    9 KB (1,200 words) - 17:18, 12 October 2023
  • The first few tutorials provided us with a spectral line data cube and a continuum image. Next we'd like to ImageMetaData Spectral reference : LSRK
    10 KB (1,203 words) - 14:28, 6 April 2022
  • The first few tutorials provided us with a spectral line data cube and a continuum image. Next we'd like to ImageMetaData Spectral reference : LSRK
    10 KB (1,203 words) - 14:46, 25 October 2022
  • [[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.]]
    9 KB (1,497 words) - 11:22, 29 May 2012
  • ...Imaging]]''' This page performs continuum subtraction and creates spectral line cubes using the MS created in [[Imaging_Prep | Prepare the data for imaging ...ctral_Line_Calibration_IRC%2B10216#How_to_Use_This_casaguide EVLA Spectral Line Calibration page for IRC+10216] page for tips on using CASA and ways CASA c
    7 KB (1,100 words) - 19:50, 12 September 2023
  • ..._IRC%2B10216_part1 Carbon Star IRC+10216: high frequency (36GHz), spectral line data reduction]. You can use this as well if you would like identical resu ...asks. One such task is {{browsetable}}, which can be run from the command line using <tt>casabrowser</tt> or within CASA as <tt>browsetable</tt>. This ta
    8 KB (1,344 words) - 15:06, 9 August 2012

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