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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 a
    44 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 directories
    20 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 a
    53 KB (8,386 words) - 15:14, 19 July 2017
  • ...The second spectral window is centered at 6668 MHz for the methanol maser line. * Spectral line projects requiring fringe-rate mapping — Fringe-rate mapping is not y
    10 KB (1,488 words) - 14:42, 1 February 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 directories
    20 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

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 sta
    3 KB (544 words) - 11:41, 9 July 2015

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