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  • ...surement sets within the ALMA pipeline: uid*targets.ms for the continuum + line (non-continuum-subtracted) target-only data, and uid*targets_line.ms to ref ...this measurement set could no longer be used with pipeline tasks, and the spectral window numbering was lost, which made it difficult to compare against the p
    12 KB (1,511 words) - 11:50, 20 October 2023
  • ...nsity contours, change the color of the vectors by selecting a different ''Line color'' (red might be a good choice). == Spectral Index Imaging ==
    29 KB (4,851 words) - 12:30, 9 April 2012
  • [[Category:ALMA]][[Category:Calibration]][[Category:Spectral Line]] *There are a lot of spectral windows! Don't be alarmed. In ALMA data,
    49 KB (7,548 words) - 15:38, 9 May 2012
  • ** [[Selecting Spectral Windows and Channels]] [http://www.splatalogue.net Splatalogue - Astronomical Line Database]
    6 KB (845 words) - 11:21, 18 July 2017
  • ...c corrections. These VLA standard calibrators, however, exhibit a negative spectral index and are relatively weak at high frequencies. ...error in the bandpass calibration. This tutorial describes how to model a spectral slope and how to correct the bandpass solution for this effect.
    28 KB (3,769 words) - 11:37, 10 July 2019
  • ...c corrections. These VLA standard calibrators, however, exhibit a negative spectral index and are relatively weak at high frequencies. ...error in the bandpass calibration. This tutorial describes how to model a spectral slope and how to correct the bandpass solution for this effect.
    28 KB (3,783 words) - 13:04, 13 November 2020
  • ...c corrections. These VLA standard calibrators, however, exhibit a negative spectral index and are relatively weak at high frequencies. ...error in the bandpass calibration. This tutorial describes how to model a spectral slope and how to correct the bandpass solution for this effect.
    26 KB (3,524 words) - 10:41, 14 June 2016
  • ...c corrections. These VLA standard calibrators, however, exhibit a negative spectral index and are relatively weak at high frequencies. ...error in the bandpass calibration. This tutorial describes how to model a spectral slope and how to correct the bandpass solution for this effect.
    26 KB (3,524 words) - 13:14, 20 April 2017
  • ...c corrections. These VLA standard calibrators, however, exhibit a negative spectral index and are relatively weak at high frequencies. ...error in the bandpass calibration. This tutorial describes how to model a spectral slope and how to correct the bandpass solution for this effect.
    26 KB (3,524 words) - 11:47, 18 November 2016
  • ...c corrections. These VLA standard calibrators, however, exhibit a negative spectral index and are relatively weak at high frequencies. ...error in the bandpass calibration. This tutorial describes how to model a spectral slope and how to correct the bandpass solution for this effect.
    29 KB (3,922 words) - 11:40, 2 May 2022
  • This casa guide covers imaging of both continuum and spectral lines of IRAS16293 Band 9. '''This guide requires CASA 5.1.1'''. In this ca ...that everything is ok. Make sure there are 4 observations, 7 fields, and 4 spectral windows (spws).
    36 KB (5,365 words) - 10:23, 28 September 2018
  • This casa guide covers imaging of both continuum and spectral lines of IRAS16293 Band 9. '''This guide requires CASA 5.6.1'''. In this ca ...that everything is ok. Make sure there are 4 observations, 7 fields, and 4 spectral windows (spws).
    36 KB (5,329 words) - 11:03, 27 October 2020
  • cs.setreferencevalue("230GHz",'spectral') cs.setincrement('1GHz','spectral')
    12 KB (1,923 words) - 13:13, 6 September 2017
  • ...n the calibrated pipeline uv-data in the DATA column, and only the science spectral window ids (spws), though importantly the spws have been re-indexed to star ...ubtraction, continuum (specmode='cont') image for aggregate spws excluding line channels identified by hif_findcont task and linecube (specmode='cube') ima
    8 KB (1,160 words) - 10:05, 8 February 2024
  • This casa guide covers imaging of both continuum and spectral lines of IRAS16293 Band 9. '''This guide requires CASA 5.4.0'''. In this ca ...that everything is ok. Make sure there are 4 observations, 7 fields, and 4 spectral windows (spws).
    37 KB (5,453 words) - 16:43, 11 March 2021
  • ...c corrections. These VLA standard calibrators, however, exhibit a negative spectral index and are relatively weak at high frequencies. ...error in the bandpass calibration. This tutorial describes how to model a spectral slope and how to correct the bandpass solution for this effect.
    27 KB (3,594 words) - 18:15, 20 July 2017
  • This casa guide covers imaging of both continuum and spectral lines of IRAS16293 Band 9. '''This guide requires CASA 5.7.0'''. In this ca ...that everything is ok. Make sure there are 4 observations, 7 fields, and 4 spectral windows (spws).
    37 KB (5,464 words) - 11:16, 10 June 2021
  • This casa guide covers imaging of both continuum and spectral lines of IRAS16293 Band 9. '''This guide requires CASA 6.1.1'''. In this ca ...that everything is ok. Make sure there are 4 observations, 7 fields, and 4 spectral windows (spws).
    37 KB (5,482 words) - 16:40, 10 June 2021
  • [[Category:ALMA]][[Category:Calibration]][[Category:Spectral Line]] *There are a lot of spectral windows! Don't be alarmed. In ALMA data,
    52 KB (7,967 words) - 17:18, 16 December 2011
  • ...c corrections. These VLA standard calibrators, however, exhibit a negative spectral index and are relatively weak at high frequencies. ...error in the bandpass calibration. This tutorial describes how to model a spectral slope and how to correct the bandpass solution for this effect.
    27 KB (3,654 words) - 14:39, 6 November 2018

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