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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+10216.84 KB (13,072 words) - 21:45, 25 April 2013
- [[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
- [[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
- #REDIRECT [[VLA high frequency Spectral Line tutorial - IRC+10216-CASA4.6]]75 bytes (10 words) - 16:25, 6 May 2016
- [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] This tutorial describes the data reduction for two spectral lines observed toward the AGB star IRC+10216.53 KB (8,284 words) - 01:44, 19 January 2012
- 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
- [[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
- [[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
- [[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
- [[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
- [[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.wi98 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 detection57 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.wi108 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 detection53 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.wi108 KB (16,739 words) - 15:08, 15 October 2020
Page text matches
- [[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 experimenting10 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 all5 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: two8 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: two9 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 : LSRK9 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 : LSRK10 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 : LSRK10 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 c7 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 ta8 KB (1,344 words) - 15:06, 9 August 2012