Search results
From CASA Guides
Jump to navigationJump to search
Page title matches
- This category contains examples of spectral line imaging in CASA, irrespective of telescope.132 members (0 subcategories, 0 files) - 10:49, 23 February 2010
File:Spectral line picker.png (2,001 × 909 (118 KB)) - 10:47, 2 May 2018- [[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
- 78 bytes (11 words) - 13:00, 23 February 2010
- ...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
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
File:MKN6 SpectralProfile.png ...profile for MKN 6 in the 2nd spectral window, spw = 1. The weak absorption line can be seen around channel 15.(881 × 522 (138 KB)) - 17:23, 25 January 2023- #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
File:MG0414 Plotants.png Plotants plot for MG0414 data set P-band spectral line CASA guide(869 × 620 (31 KB)) - 17:39, 24 April 2018- #REDIRECT [[HI 21cm (1.4 GHz) spectral line data reduction: LEDA 44055-CASA6.5.2]]82 bytes (10 words) - 19:27, 16 November 2022
- This category contains examples of spectral line imaging in CASA, irrespective of telescope.132 members (0 subcategories, 0 files) - 10:49, 23 February 2010
File:AmpVfreq colorspw.png .../submm guide: SMA line data. To demonstrate that there is overlap between spectral windows. Plotms of amplitude vs frequency, averaged over time, scan, basel(869 × 649 (87 KB)) - 17:30, 14 October 2010- * 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
File:MG0414 d1 Plotants zoomedin.png Plotants plot of MG0414 data set P-band spectral line CASA guide zoomed in to show center of Y w/ location of the refant ea04(622 × 461 (20 KB)) - 17:40, 24 April 2018
