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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. This carbon star, which is a44 KB (6,777 words) - 12:19, 19 May 2010
- #REDIRECT [[CARMA spectral line mosaic M99 3.1]]48 bytes (6 words) - 17:27, 26 May 2011
- ...dy of M99). The velocity of the gas, traced by the doppler shift of the CO line, can be used to measure the total mass of the galaxy (including dark matter ...ze a wide band (500 MHz) spectral window to calibrate narrow band (60 MHz) spectral windows in order to achieve better signal-to-noise.37 KB (5,752 words) - 17:27, 26 May 2011
- [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] This tutorial describes the data reduction for two spectral lines observed toward the AGB star IRC+10216.45 KB (7,121 words) - 14:11, 21 May 2012
- ...dy of M99). The velocity of the gas, traced by the doppler shift of the CO line, can be used to measure the total mass of the galaxy (including dark matter ...ze a wide band (500 MHz) spectral window to calibrate narrow band (60 MHz) spectral windows in order to achieve better signal-to-noise.39 KB (6,041 words) - 13:04, 5 July 2011
- ...ITS files. The following variables could be defined either on the command line inside CASA, or in an executable python script: "c0104I.4.ms" .) The following lines then concatenate the individual spectral windows MS directories20 KB (3,309 words) - 17:30, 16 March 2012
- This tutorial picks up where [[EVLA Spectral Line Calibration IRC+10216]] leaves off. [[Image:irc10216_uvspec.png|thumb|UV-plot of the spectral line signal in both spw for IRC+10216.]]21 KB (3,516 words) - 16:03, 2 September 2011
- [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] This tutorial describes the data reduction for two spectral lines observed toward the AGB star IRC+10216.49 KB (7,632 words) - 21:16, 29 August 2011
- ...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 (1,853 words) - 13:35, 9 January 2012
- NEW P-BAND SPECTRAL LINE GUIDE. BELOW IS A COPY of P-BAND CONTINUUM on the (linux) command line. This should start a CASA interactive python (iPython) session, and open a53 KB (8,386 words) - 15:14, 19 July 2017
- ...ded into 256 spectral channels centered at 6668 MHz for the methanol maser line. * Spectral line projects requiring fringe-rate mapping — Fringe-rate mapping is not y21 KB (3,417 words) - 16:56, 30 April 2024
- ...ITS files. The following variables could be defined either on the command line inside CASA, or in an executable python script: "c0104I.4.ms" .) The following lines then concatenate the individual spectral windows MS directories20 KB (3,312 words) - 14:21, 6 October 2010
- #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 AGB star IRC+10216.53 KB (8,230 words) - 18:47, 17 May 2012
- 79 bytes (11 words) - 10:04, 16 October 2020
- [[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
- ...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
- 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
- #REDIRECT [[EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.6]]76 bytes (10 words) - 16:22, 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+10216.81 KB (12,845 words) - 16:03, 1 June 2012
- [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] This tutorial describes the data reduction for two spectral lines observed toward the AGB star IRC+10216.81 KB (12,853 words) - 22:34, 6 December 2012
- [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] This tutorial describes the data reduction for two spectral lines observed toward the AGB star IRC+10216.82 KB (13,029 words) - 16:14, 30 May 2013
- #REDIRECT [[EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.0]]76 bytes (10 words) - 19:31, 22 October 2012
- [[Category:EVLA]][[Category:Calibration]][[Category:Spectral Line]] This tutorial describes the data reduction for two spectral lines observed toward the AGB star IRC+10216.84 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
- * 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 sta3 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 experimenting9 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 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