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  • [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] This tutorial describes the data reduction for two spectral lines observed toward the AGB star IRC+10216.
    83 KB (13,072 words) - 19:38, 4 February 2014
  • [[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.
    90 KB (14,142 words) - 18:38, 10 March 2016
  • [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] This tutorial describes the data reduction for two spectral lines observed toward the AGB star IRC+10216.
    83 KB (13,039 words) - 18:00, 20 July 2015
  • [[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 (14,512 words) - 17:26, 25 May 2017
  • #REDIRECT [[VLA high frequency Spectral Line tutorial - IRC+10216-CASA4.7]]
    75 bytes (10 words) - 20:00, 17 November 2016
  • [[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 [https://en.wi
    98 KB (15,214 words) - 11:44, 3 October 2018
  • This tutorial describes how to use CASA 5.0.0 to reduce spectral-line data in the low-frequency P-band of the VLA (230–470 MHz). The goal i * Additionally, if very high spectral dynamic range is needed (i.e., when expecting a ratio between the detection
    57 KB (8,166 words) - 15:22, 22 October 2018
  • [[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 [https://en.wi
    108 KB (16,694 words) - 10:46, 11 June 2019
  • This tutorial describes how to use CASA 5.4.0 to reduce spectral-line data in the low-frequency P-band of the VLA (230–470 MHz). The goal i * Additionally, if very high spectral dynamic range is needed (i.e., when expecting a ratio between the detection
    53 KB (7,739 words) - 10:46, 25 April 2019
  • [[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 [https://en.wi
    108 KB (16,739 words) - 15:08, 15 October 2020
  • This tutorial describes how to use CASA 5.5.0 to reduce spectral-line data in the low-frequency P-band of the VLA (230–470 MHz). The goal i * Additionally, if very high spectral dynamic range is needed (i.e., when expecting a ratio between the detection
    53 KB (7,864 words) - 12:50, 29 September 2020
  • [[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 [https://en.wi
    108 KB (16,776 words) - 15:14, 15 October 2020
  • This tutorial describes how to use CASA 5.7.2 to reduce spectral-line data in the low-frequency P-band of the VLA (230–470 MHz). The goal i * Additionally, if very high spectral dynamic range is needed (i.e., when expecting a ratio between the detection
    57 KB (8,502 words) - 18:49, 22 December 2020
  • #REDIRECT [[MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.4]]
    68 bytes (8 words) - 17:52, 29 February 2024
  • [[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 [https://en.wi
    119 KB (18,324 words) - 12:17, 24 February 2023
  • This tutorial describes how to use CASA 6.2.0 to reduce spectral-line data in the low-frequency P-band of the VLA (230–470 MHz). The goal i * Additionally, if very high spectral dynamic range is needed (i.e., when expecting a ratio between the detection
    63 KB (9,411 words) - 23:23, 12 February 2023
  • [[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 [https://en.wi
    119 KB (18,324 words) - 14:03, 2 March 2023
  • This tutorial describes how to use CASA 6.5.2 to reduce spectral-line data in the low-frequency P-band of the VLA (230–470 MHz). The goal i * Additionally, if very high spectral dynamic range is needed (i.e., when expecting a ratio between the detection
    66 KB (9,867 words) - 13:55, 24 January 2024
  • #REDIRECT [[MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.2]]
    68 bytes (8 words) - 15:35, 13 February 2023
  • [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] ...w to calibrate and image high-frequency (Ka Band) EVLA observations of two spectral lines toward the Asymptotic Giant Branch (AGB) star [https://en.wikipedia.o
    134 KB (19,330 words) - 16:53, 29 September 2023

Page text matches

  • 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
  • ...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
    15 KB (2,458 words) - 16:48, 7 June 2016
  • == Continuum Subtraction for Line Emission == ...do not need to continuum subtract if the line of interest is an absorption line.
    16 KB (2,477 words) - 16:36, 28 February 2024
  • [[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
    9 KB (1,443 words) - 12:08, 22 November 2011
  • [[Category:ALMA]][[Category:Calibration]][[Category:Spectral Line]] available basebands, which are associated with four different spectral windows: two
    9 KB (1,395 words) - 09:09, 7 September 2015
  • ...t look at spectral line imaging]]: This guide shows imaging of a spectral line. ...t spectral line imaging in CASA]]: This guide shows imaging of a spectral line.
    8 KB (1,160 words) - 16:55, 13 May 2024
  • [[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 (1,372 words) - 22:05, 9 January 2017
  • ** [[Selecting Spectral Windows and Channels]] ** <big> [http://www.splatalogue.net Splatalogue - Astronomical Line Database] </big>
    3 KB (404 words) - 00:19, 18 November 2017
  • * A first look at spectral line imaging: [[First_Look_at_Line_Imaging_4.4 | CASA 4.4]] [[First_Look_at_Line
    2 KB (320 words) - 17:19, 12 October 2023
  • == Continuum Subtraction for Line Emission == ...do not need to continuum subtract if the line of interest is an absorption line.
    16 KB (2,499 words) - 15:03, 18 October 2023
  • [[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
    10 KB (1,605 words) - 11:54, 30 May 2012

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