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- ...ry high spectral resolution centered on the maser line. The methanol maser line itself has a rest frequency of 6668.5192 MHz (e.g., [https://ui.adsabs.harv ...m the primary file to the zoom file, target imaging, and specific spectral line analysis steps. ...112 KB (16,338 words) - 20:41, 23 September 2024
- 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) - 19:14, 19 July 2017
- [[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) - 01:16, 30 August 2011
- 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) - 20:03, 2 September 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) - 17:35, 9 January 2012
- #REDIRECT [[MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.4]] ...68 bytes (8 words) - 21:52, 29 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) - 18:21, 6 October 2010
- [[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) - 20:14, 30 May 2013
- 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) - 21:46, 6 January 2012
- #REDIRECT [[EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.0]] ...76 bytes (10 words) - 23:31, 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) - 01:45, 26 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. ...53 KB (8,230 words) - 22:47, 17 May 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 (12,857 words) - 17:35, 2 June 2015
- 79 bytes (11 words) - 14:04, 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) - 00:37, 1 March 2012
- #REDIRECT [[EVLA high frequency Spectral Line tutorial - IRC+10216-CASA4.6]] ...76 bytes (10 words) - 20:22, 6 May 2016
- ...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) - 21:57, 6 January 2012
Page text matches
- #REDIRECT [[MG0414+0534 P-band Spectral Line Tutorial - CASA 6.5.4]] ...68 bytes (8 words) - 21:52, 29 February 2024
- #REDIRECT [[HI 21cm (1.4 GHz) spectral line data reduction: LEDA 44055]] ...72 bytes (9 words) - 22:04, 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) - 18:22, 16 January 2012
- #REDIRECT [[HI 21cm (1.4 GHz) spectral line data reduction: LEDA 44055-CASA6.5.2]] ...82 bytes (10 words) - 23:27, 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) - 23:16, 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) - 21:46, 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) - 02:04, 24 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) - 16:03, 1 March 2024
- first look at spectral line imaging: ...891 bytes (116 words) - 21:46, 18 July 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) - 22:09, 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) - 15:41, 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) - 15:13, 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) - 05:21, 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) - 15:18, 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) - 20:45, 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 experimenting ...9 KB (1,578 words) - 14:49, 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) - 21:24, 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) - 19:05, 29 May 2019
