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  • EVLA spectral line IRC10216
    [[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
  • CARMA spectral line mosaic M99
    #REDIRECT [[CARMA spectral line mosaic M99 3.1]]
    48 bytes (6 words) - 17:27, 26 May 2011
  • CARMA spectral line mosaic M99 3.1
    ...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
  • EVLA Spectral Line Calibration IRC+10216
    [[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
  • CARMA spectral line mosaic M99 3.2
    ...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
  • Calibrating a Mosaicked Spectral Line Dataset
    ...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
  • EVLA Spectral Line Imaging Analysis IRC+10216
    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
  • EVLA Spectral Line Calibration IRC+10216 - workshop
    [[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
  • EVLA high frequency Spectral Line Tutorial - CDE
    ...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
  • P-band spectral line tutorial-CASA5.0.0
    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
  • VLBA Basic Spectral Line Tutorial DRAFT
    ...ded into 256 spectral channels centered at 6668 MHz for the methanol maser line. ...and spectral line projects are in the target imaging and specific spectral line analysis steps.
    52 KB (8,358 words) - 18:00, 14 May 2024
  • Importing and Calibrating a Mosaicked Spectral Line Dataset
    ...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
  • MG0414+0534 P-band Spectral Line Tutorial
    #REDIRECT [[MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.4]]
    68 bytes (8 words) - 17:52, 29 February 2024
  • EVLA high frequency Spectral Line tutorial - IRC+10216 part1
    [[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
  • VLA high frequency Spectral Line tutorial - IRC+10216
    79 bytes (11 words) - 10:04, 16 October 2020
  • EVLA high frequency Spectral Line tutorial - IRC+10216 part2
    [[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
  • EVLA high frequency spectral line tutorial - IRC+10216 - calibration
    ...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
  • EVLA high frequency spectral line tutorial - IRC+10216 - imaging
    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
  • EVLA high frequency Spectral Line tutorial - IRC+10216
    #REDIRECT [[EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.6]]
    76 bytes (10 words) - 16:22, 6 May 2016
  • EVLA high frequency Spectral Line tutorial - IRC+10216 CASA3.4
    [[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
  • EVLA high frequency Spectral Line tutorial - IRC+10216-CASA3.4
    [[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
  • EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.0
    [[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
  • EVLA high frequency Spectral Line tutorial - IRC+10216-CAS4.0
    #REDIRECT [[EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.0]]
    76 bytes (10 words) - 19:31, 22 October 2012
  • EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.1.0
    [[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
  • EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.3
    [[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
  • EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.4
    [[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
  • EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.6
    #REDIRECT [[VLA high frequency Spectral Line tutorial - IRC+10216-CASA4.6]]
    75 bytes (10 words) - 16:25, 6 May 2016
  • EVLA high frequency Spectral Line tutorial - IRC+10216 part1 (Caltech)
    [[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
  • EVLA high frequency Spectral Line tutorial - IRC+10216 part2 (Caltech)
    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
  • EVLA high frequency Spectral Line tutorial - IRC+10216 part1-CASA3.3
    [[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
  • EVLA high frequency Spectral Line tutorial - IRC+10216 part2-CASA3.3
    [[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
  • VLA high frequency Spectral Line tutorial - IRC+10216-CASA4.6
    [[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
  • EVLA high frequency Spectral Line tutorial - IRC+10216 - CASA 4.2
    [[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
  • EVLA high frequency Spectral Line tutorial - IRC+10216 - CASA 4.1
    [[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
  • EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.5
    [[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
  • EVLA high frequency Spectral Line tutorial - IRC+10216-newfile
    [[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
  • VLA high frequency Spectral Line tutorial - IRC+10216-CASA4.7
    [[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
  • EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.7
    #REDIRECT [[VLA high frequency Spectral Line tutorial - IRC+10216-CASA4.7]]
    75 bytes (10 words) - 20:00, 17 November 2016
  • VLA high frequency Spectral Line tutorial - IRC+10216-CASA5.0.0
    [[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
  • MG0414+0534 P-band Spectral Line Tutorial - CASA 5.0.0
    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
  • VLA high frequency Spectral Line tutorial - IRC+10216-CASA5.4.0
    [[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
  • MG0414+0534 P-band Spectral Line Tutorial - CASA 5.4.0
    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
  • VLA high frequency Spectral Line tutorial - IRC+10216-CASA5.5.0
    [[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
  • MG0414+0534 P-band Spectral Line Tutorial - CASA 5.5.0
    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
  • VLA high frequency Spectral Line tutorial - IRC+10216-CASA5.7.0
    [[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
  • MG0414+0534 P-band Spectral Line Tutorial - CASA 5.7.2
    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
  • MG0414+0534 P-band Spectral Line Tutorial - CASA 5.7.0
    #REDIRECT [[MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.4]]
    68 bytes (8 words) - 17:52, 29 February 2024
  • VLA high frequency Spectral Line tutorial - IRC+10216-CASA6.2.0
    [[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
  • MG0414+0534 P-band Spectral Line Tutorial - CASA 6.2.0
    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
  • VLA high frequency Spectral Line tutorial - IRC+10216-CASA6.4.1
    [[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
  • MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.2
    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
  • MG0414+0534 P-band Spectral Line Tutorial - CASA 6.4.1
    #REDIRECT [[MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.2]]
    68 bytes (8 words) - 15:35, 13 February 2023
  • VLA high frequency Spectral Line tutorial - IRC+10216-CASA6.5.3
    [[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
  • MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.4 MG0414 0534 P-band Spectral Line Tutorial (CASA 6.5.4)
    This tutorial describes how to use CASA 6.5.4 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 (9,882 words) - 11:21, 29 February 2024
  • MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.4
    This tutorial describes how to use CASA 6.5.4 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 (9,882 words) - 14:06, 29 February 2024
  • HI 21cm (1.4 GHz) spectral line data reduction: LEDA 44055
    This tutorial describes the data reduction of the HI spectral line observed of the nearby (4.8 Mpc), gas-rich dwarf galaxy LEDA44055. For its ...rvation, a 16 MHz wide IF pair (A0C0 as seen in later in listobs) subband (spectral window, abbreviated as ''spw'' in CASA) using 4096 channels was observed, e
    79 KB (10,810 words) - 18:24, 14 February 2020
  • HI 21cm (1.4 GHz) spectral line data reduction: LEDA 44055-CASA5.7.0
    This tutorial describes the data reduction of the HI spectral line observed of the nearby (4.8 Mpc), gas-rich dwarf galaxy LEDA44055. For its ...rvation, a 16 MHz wide IF pair (A0C0 as seen in later in listobs) subband (spectral window, abbreviated as ''spw'' in CASA) using 4096 channels was observed, e
    79 KB (10,809 words) - 14:21, 9 April 2021
  • HI 21cm (1.4 GHz) spectral line data reduction: LEDA 44055-CASA6.2.0
    This tutorial describes the data reduction of the HI spectral line observed of the nearby (4.8 Mpc), gas-rich dwarf galaxy LEDA44055. For its ...rvation, a 16 MHz wide IF pair (A0C0 as seen in later in listobs) subband (spectral window, abbreviated as ''spw'' in CASA) using 4096 channels was observed, e
    85 KB (11,808 words) - 11:37, 2 May 2022
  • HI 21cm (1.4 GHz) spectral line data reduction: LEDA 44055-CASA6.5.2
    This tutorial describes the data reduction of the HI spectral line observed of the nearby (4.8 Mpc), gas-rich dwarf galaxy LEDA44055. For its ...rvation, a 16 MHz wide IF pair (A0C0 as seen in later in listobs) subband (spectral window, abbreviated as ''spw'' in CASA) using 4096 channels was observed, e
    91 KB (12,686 words) - 20:32, 20 February 2024
  • HI 21cm (1.4 GHz) spectral line data reduction: LEDA 44055-CASA6.4.1
    #REDIRECT [[HI 21cm (1.4 GHz) spectral line data reduction: LEDA 44055-CASA6.5.2]]
    82 bytes (10 words) - 19:27, 16 November 2022

Page text matches

  • Current MM/Submm Guides
    * 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
  • Past MM/Submm Guides
    * 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
  • EVLA high frequency Spectral Line tutorial - IRC+10216-CAS4.0
    #REDIRECT [[EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.0]]
    76 bytes (10 words) - 19:31, 22 October 2012
  • EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.6
    #REDIRECT [[VLA high frequency Spectral Line tutorial - IRC+10216-CASA4.6]]
    75 bytes (10 words) - 16:25, 6 May 2016
  • EVLA high frequency Spectral Line tutorial - IRC+10216
    #REDIRECT [[EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.6]]
    76 bytes (10 words) - 16:22, 6 May 2016
  • EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.7
    #REDIRECT [[VLA high frequency Spectral Line tutorial - IRC+10216-CASA4.7]]
    75 bytes (10 words) - 20:00, 17 November 2016
  • MG0414 Pband Tutorial
    #REDIRECT [[MG0414+0534 P-band Spectral Line Tutorial - CASA 5.0.0]]
    68 bytes (8 words) - 13:32, 2 September 2017
  • MG0414+0534 P-band Spectral Line Tutorial
    #REDIRECT [[MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.4]]
    68 bytes (8 words) - 17:52, 29 February 2024
  • MG0414+0534 P-band Spectral Line Tutorial - CASA 5.7.0
    #REDIRECT [[MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.4]]
    68 bytes (8 words) - 17:52, 29 February 2024
  • MG0414+0534 P-band Spectral Line Tutorial - CASA 6.4.1
    #REDIRECT [[MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.2]]
    68 bytes (8 words) - 15:35, 13 February 2023
  • TDEM0025 HI tutorial
    #REDIRECT [[HI 21cm (1.4 GHz) spectral line data reduction: LEDA 44055]]
    72 bytes (9 words) - 18:04, 4 February 2019
  • Caltech CASA Tutorials
    * 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
  • HI 21cm (1.4 GHz) spectral line data reduction: LEDA 44055-CASA6.4.1
    #REDIRECT [[HI 21cm (1.4 GHz) spectral line data reduction: LEDA 44055-CASA6.5.2]]
    82 bytes (10 words) - 19:27, 16 November 2022
  • Pre-upgrade VLA Tutorials
    * 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
  • EVLA high frequency spectral line tutorial - IRC+10216 - imaging
    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
  • Stacking Multiple Spectral Lines at Same Position
    ...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
  • Karl G. Jansky VLA Tutorials-archived
    ...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
  • NewPage
    ...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
  • Create a Clean Mask from Continuum Image or Moment Cube
    ...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
  • First Look at Line Imaging 4.4
    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
  • Spectral Viewer
    <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
  • First Look at Image Analysis 4.4
    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
  • List of All Tutorials
    ...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
  • WorkshopSelfcal
    ...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 experimenting
    9 KB (1,578 words) - 10:49, 27 February 2013
  • Karl G. Jansky VLA Tutorials
    ...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
  • First Look at Line Imaging CDE
    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
  • TWHydraBand7 for CASA 3.4 defunct
    [[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
  • TWHydraBand7 For CASA 3.3
    [[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
  • TWHydraBand7 For CASA 3.4
    [[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
  • WorkshopSelfcal (Caltech)
    ...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 experimenting
    10 KB (1,646 words) - 03:38, 18 January 2012
  • First Look at Line Imaging CASA 5.7
    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
  • Notes on EVLA OSRO continuum data sets
    ..._the_Bandpasses | bandpass calibration]], just as you would for a spectral line data set; and spw = '' # Spectral windows e.g. '0~3', '' is all
    5 KB (667 words) - 14:05, 25 March 2010
  • First Look at Line Imaging CASA 6
    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
  • First Look at Line Imaging CASA 6.4
    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
  • NGC3256Band3 for CASA 3.3
    [[Category:ALMA]][[Category:Calibration]][[Category:Spectral Line]] available basebands, which are associated with four different spectral windows: two
    8 KB (1,256 words) - 10:57, 26 April 2012
  • Initial instructions for 2010
    ** 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
  • TWHydraBand7 (Caltech)
    [[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
  • First Look at Line Imaging CASA 6.5.4
    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
  • NGC3256Band3 (Caltech)
    [[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
  • First Look at Image Analysis CDE
    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
  • Guide to the NA Imaging Template
    ...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
  • First Look at Image Analysis CASA 5.7
    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
  • First Look at Image Analysis CASA 6
    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
  • First Look at Image Analysis CASA 6.4
    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
  • TWHydraBand7 SS12 Overview
    [[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
  • Guide to the NA Imaging Template CASA 6.5.4
    ...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
  • Measurement Set Contents
    ..._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
  • OT tutorial SISS
    ...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
  • Image Line CASA 6.1.1
    == 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
  • AntennaeBand7 for CASA 3.3
    [[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
  • NGC3256Band3
    [[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
  • ALMAguides
    ...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
  • TWHydraBand7
    [[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
  • CASA Tips
    ** [[Selecting Spectral Windows and Channels]] ** <big> [http://www.splatalogue.net Splatalogue - Astronomical Line Database] </big>
    3 KB (404 words) - 00:19, 18 November 2017
  • Archived ALMA CASAguides
    * 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
  • Image Line CASA 6.5.4
    == 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
  • AntennaeBand7 3.4
    [[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
  • First Look at Image Analysis CASA 6.5.4
    The first few tutorials provided us with a spectral line data cube and a continuum image. Next we'd like to ...e extracted script and you want to use your own images from completing the line imaging tutorial
    12 KB (1,674 words) - 10:15, 8 February 2024
  • What is CASA?
    ...data table is arranged so that each row is a single timestamp for a single spectral window and a single baseline. There are several columns. DATA holds the ori * {{uvcontsub}}: carry out uv-plane continuum subtraction for spectral-line data
    6 KB (862 words) - 17:03, 27 March 2013
  • EVLA Spectral Line Imaging Analysis IRC+10216
    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
  • CASA Contributed Script: plotweather
    ...he MS (see example below) as well as estimate the zenith opacity for each spectral window. This script is only intended for use with the EVLA-- it contains h #edit the last line of the script, replacing MSname.ms with the name of your measurement set, a
    2 KB (344 words) - 13:26, 13 December 2012
  • WorkshopImaging
    ...s here (about 15 MHz per channel). The spectral windows cover the CO J=1-0 line, a CN doublet, and the 3mm continuum. All three types of emission are visib ...ode) and cover the 850 micron continuum, the CO J=3-2 line, and HCO+ J=4-3 line. There is a full CASA Guide describing the reduction and imaging of these d
    21 KB (3,592 words) - 16:03, 26 February 2013
  • Spectralindex
    ...as the first argument in order to determine the center frequencies of each spectral window. (To avoid the need for this file in the future, we have submitted ...y, it produces a plot summarizing the results. By default, it will use all spectral windows, but it will exclude those with an "INSUFFICIENT DATA" status from
    8 KB (1,058 words) - 12:56, 8 August 2013
  • EVLA high frequency spectral line tutorial - IRC+10216 - calibration
    ...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
  • EVLA high frequency Spectral Line Tutorial - CDE
    ...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
  • Combining Bandpasses
    ...mes the bandpass calibrator at the required frequency is contaminated with line absorption or emission. In particular, this is notorious for observations c ...bserving frequency. The offset frequencies should be chosen clean from any line contamination, but with as little frequency offset as possible. Ideally it
    10 KB (1,205 words) - 15:47, 11 March 2021
  • ALMA2014 LBC SVDATA
    ...iate amount of channel averaging has been applied to reduce the data size. Line data sets are provided at their full resolution. If self-calibration was po ...the primary beam images themselves and can be applied to the corresponding line data if desired using the CASA task {{impbcor}}.
    16 KB (2,452 words) - 10:11, 8 May 2018
  • VLBI Tutorials
    ...[https://casaguides.nrao.edu/index.php/AIPS-Spectral_Lines_and_Astrometry Spectral Lines and Astrometry] ...//www.jb.man.ac.uk/DARA/unit4/Workshops/Spectral_line.html EVN HI Spectral Line]
    4 KB (593 words) - 18:09, 2 June 2023
  • ALMAguides old
    ...at spectral line imaging in CASA]] This guide shows imaging of a spectral line.
    6 KB (859 words) - 16:29, 8 January 2018
  • NGC3256 Band3 - Imaging (Caltech)
    [[Category:ALMA]][[Category:Imaging]][[Category:Spectral Line]] ...tech)]]''' CASA Guide will cover the imaging of the continuum and spectral line data. It begins where the '''[[NGC3256 Band3 - Calibration (Caltech)]]'''
    24 KB (3,568 words) - 21:20, 12 January 2012
  • NGC3256 Band3 - Imaging for CASA 3.3
    [[Category:ALMA]][[Category:Imaging]][[Category:Spectral Line]] ...Band3]]''' CASA Guide will cover the imaging of the continuum and spectral line data. It begins where the '''[[NGC3256 Band3 - Calibration]]''' section le
    24 KB (3,580 words) - 05:18, 11 May 2012
  • What's the difference between Antenna1 and Antenna2? Axis definitions in plotms
    ...r (analogous to what VLA users know as an IF). The characteristics of each spectral window are listed in {{listobs}}. * the rest frequency of the spectral line.
    5 KB (842 words) - 18:01, 7 June 2010
  • ADMIT Products and Usage CASA 5.4.0
    ...tify spectral features, and create moment maps of each identified spectral line. ...s using the online version of Splatalogue rather than the internal one for line identification. These can be tuned via creating a file with your parameter
    15 KB (2,623 words) - 16:10, 28 February 2024
  • NGC3256 Band3 Imaging for CASA 4.1
    [[Category:ALMA]][[Category:Imaging]][[Category:Spectral Line]] ...SA Guide for CASA 4.1 will cover the imaging of the continuum and spectral line data. It begins where the '''[[NGC3256 Band3 Calibration for CASA 4.1]]'''
    24 KB (3,681 words) - 09:10, 19 April 2013
  • NGC3256 Band3 Imaging for CASA 3.4
    [[Category:ALMA]][[Category:Imaging]][[Category:Spectral Line]] ...SA Guide for CASA 3.4 will cover the imaging of the continuum and spectral line data. It begins where the '''[[NGC3256 Band3 Calibration for CASA 3.4]]'''
    24 KB (3,683 words) - 10:44, 1 June 2012
  • NGC3256 Band3 Imaging for CASA 4.0
    [[Category:ALMA]][[Category:Imaging]][[Category:Spectral Line]] ...SA Guide for CASA 4.0 will cover the imaging of the continuum and spectral line data. It begins where the '''[[NGC3256 Band3 Calibration for CASA 4.0]]'''
    24 KB (3,681 words) - 13:14, 27 October 2012
  • AntennaeBand7 North SS12
    [[Category:ALMA]][[Category:Calibration]][[Category:Spectral Line]] ...426 km/s); because the data are automatically Hanning smoothed, the actual spectral resolution is twice this. The TDM mode data were observed and used mainly f
    9 KB (1,381 words) - 10:20, 5 June 2012
  • NGC3256 Band3 Imaging for CASA 4.2
    [[Category:ALMA]][[Category:Imaging]][[Category:Spectral Line]] ...SA Guide for CASA 4.2 will cover the imaging of the continuum and spectral line data. It begins where the '''[[NGC3256 Band3 Calibration for CASA 4.2]]'''
    24 KB (3,712 words) - 11:47, 29 November 2013
  • HTT2
    * [[Selecting Spectral Windows and Channels]] *[[Applying EVLA on-line flags]] What do to if you need to re-apply (or apply) your online flags, wi
    3 KB (447 words) - 16:38, 30 October 2017
  • Lstrange
    ...ent. It also lists the range of elevations on the target source, and a one-line summary that can be pasted into a table on the SCOPS wikipages. Note that t Ignoring spectral window [0, 25, 26, 27, 28, 29, 30, 31, 32, 33] because it is WVR related
    2 KB (265 words) - 11:50, 1 March 2012
  • Obtaining Data: 3C 391 Example
    ...evel of time-average smearing. In this example, we opt not to perform any spectral or temporal averaging, and later show how this may be done after the fact b ...nations, particularly in compact configurations, one antenna may block the line of sight between another antenna and the source of interest. This effect i
    7 KB (1,170 words) - 16:58, 8 May 2016
  • ADMIT Products and Usage CASA 6.5.4
    ...tify spectral features, and create moment maps of each identified spectral line. ...s using the online version of Splatalogue rather than the internal one for line identification. These can be tuned via creating a file with your parameter
    16 KB (2,805 words) - 16:18, 28 February 2024
  • CASA Parallel Processing
    ...task level, <tt>pcont</tt> and <tt>pcube</tt> (for continuum and spectral line imaging, respectively). spw = '' # Select spectral window/channels
    11 KB (1,493 words) - 19:35, 8 May 2012
  • Inspecting Data
    ...12 scans of ~1.5-minute duration each with 10s integrations. There are 15 spectral windows, the first half containing RR and second half with LL polarizations ...vation was done at night (the black disk represents the sun, below the red line, which is the horizon). The second panel shows the wind speed and directio
    10 KB (1,752 words) - 14:56, 9 August 2012
  • OT tutorial SISS 2018
    ...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
    25 KB (4,152 words) - 11:36, 16 May 2018
  • AntennaeBand7
    [[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
    11 KB (1,652 words) - 04:27, 31 December 2023
  • Data flagging with viewer
    ...s''' or '''channels''', the latter being particularly helpful for spectral-line experiments. ...ll probably also want to use the DVD-style control buttons to step through spectral channels. You can change which data dimension is affected by these control
    11 KB (1,676 words) - 10:56, 20 July 2017
  • Tclean and ALMA CASA 6.5.4
    '''Specifying spectral gridding mode:''' * Specifying the the spectral gridding type in clean with "mode" (mfs, channel, velocity, frequency) is n
    12 KB (1,661 words) - 13:44, 15 March 2024
  • Calibrating M99
    * The Spectral Window ID (SpwID) of each spectral window you want to calibrate. ...e listobs output, you will find listings of the properties of the observed spectral windows, and the locations of the antennas. In this case, the narrowband wi
    12 KB (1,968 words) - 13:26, 29 April 2010
  • TCLEAN and ALMA CASA 5
    '''Specifying spectral gridding mode:''' * Specifying the the spectral gridding type in clean with "mode" (mfs, channel, velocity, frequency) is n
    12 KB (1,731 words) - 13:40, 15 March 2024
  • M100 Band3
    ....281 kHz, or 1.27 km/s, and one of the windows is centered at the CO (1-0) line with a rest frequency of 115.271 GHz in ALMA Band 3. There are three 12m da ....281 kHz, or 1.27 km/s, and one of the windows is centered at the CO (1-0) line with a rest frequency of 115.271 GHz in ALMA Band 3; this setup mirrors the
    11 KB (1,777 words) - 18:56, 26 March 2024
  • EVLA high frequency Spectral Line tutorial - IRC+10216 part2 (Caltech)
    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
  • EVLA high frequency Spectral Line tutorial - IRC+10216 part2
    [[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
  • EVLA high frequency Spectral Line tutorial - IRC+10216 part2-CASA3.3
    [[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
  • IRAS16293Band9
    [[Category:ALMA]] [[Category:Calibration]] [[Category:Spectral line]] Previous molecular line studies with the SMA have revealed detailed structure and kinematics in the
    12 KB (1,832 words) - 23:18, 30 January 2024
  • NGC3256 Band3 Imaging for CASA 4.4
    [[Category:ALMA]][[Category:Imaging]][[Category:Spectral Line]] ...SA Guide for CASA 4.4 will cover the imaging of the continuum and spectral line data. It begins where the '''[[NGC3256 Band3 Calibration for CASA 4.4]]'''
    24 KB (3,714 words) - 14:51, 4 February 2016
  • NGC3256 Band3 Imaging for CASA 4.5
    [[Category:ALMA]][[Category:Imaging]][[Category:Spectral Line]] ...SA Guide for CASA 4.5 will cover the imaging of the continuum and spectral line data. It begins where the '''[[NGC3256 Band3 Calibration for CASA 4.5]]'''
    25 KB (3,722 words) - 14:57, 4 April 2017

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