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- ...x|thumb|right|<caption>Northern mosaic: Amplitude vs. channel. The CO(3-2) line is seen from 70 to 100</caption>]] ...e found by plotting the average spectrum (all fields). We find the CO(3-2) line from channels 70 to 100 in the northern mosaic (<xr id="Antennae_North-AMPv40 KB (6,363 words) - 12:47, 5 June 2012
- [[Category:ALMA]][[Category:Imaging]][[Category:Spectral Line]] ...o an image of the sky. We will separately image continuum emission and two spectral lines, CO 3-2 and HCO+ 4-3. We will use the results of our continuum imagin47 KB (7,259 words) - 16:08, 31 May 2012
- ...d of _target.ms, comment out the previous line and uncomment the following line ...anually review the uvwave vs amp and channel vs amp plots of all field and spectral windows in the MS file. Outliers seen in the calibrator fields of these pl23 KB (2,951 words) - 13:49, 7 December 2023
- [[Category:ALMA]][[Category:Imaging]][[Category:Spectral Line]] ...nnaeBand7]]''' CASA Guide covers the imaging of the continuum and spectral line data. It begins where the '''[[Antennae Band7 - Calibration]]''' section l41 KB (6,416 words) - 16:05, 16 May 2012
- ...window for TW Hydra with channel vs amplitude. Spw 0 has a strong spectral line and spw 3 is a continuum only window.]] The first step is to identify which spectral windows (spws) you would like to include in the continuum. In general, you32 KB (5,048 words) - 14:42, 18 October 2023
- This casa guide covers imaging of both continuum and spectral lines of IRAS16293 Band 9. '''This guide requires CASA 4.4'''. In this casa Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)29 KB (4,388 words) - 21:53, 6 July 2015
- This casa guide covers imaging of both continuum and spectral lines of IRAS16293 Band 9. '''This guide requires CASA 4.3'''. In this casa Spectral Windows: (4 unique spectral windows and 1 unique polarization setups)30 KB (4,388 words) - 11:03, 21 February 2018
- ...VLA]][[Category: Calibration]] [[Category: Imaging]] [[Category: Spectral Line]] ....tclean.html tclean] includes flexible regridding and interpolation in the spectral domain. [https://casadocs.readthedocs.io/en/v6.5.2/api/tt/casatasks.imaging35 KB (5,087 words) - 17:54, 8 February 2023
- [[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
- ...anually review the uvwave vs amp and channel vs amp plots of all field and spectral windows in the MS file. Outliers seen in the calibrator fields of these pl ...alibrated directory. You can also use the GUI interface to iterate through spectral windows (spws).22 KB (2,892 words) - 16:28, 28 February 2024
- ...surement sets within the ALMA pipeline: uid*targets.ms for the continuum + line (non-continuum-subtracted) target-only data, and uid*targets_line.ms to ref ...this measurement set could no longer be used with pipeline tasks, and the spectral window numbering was lost, which made it difficult to compare against the p12 KB (1,511 words) - 11:50, 20 October 2023
- ...nsity contours, change the color of the vectors by selecting a different ''Line color'' (red might be a good choice). == Spectral Index Imaging ==29 KB (4,851 words) - 12:30, 9 April 2012
- [[Category:ALMA]][[Category:Calibration]][[Category:Spectral Line]] *There are a lot of spectral windows! Don't be alarmed. In ALMA data,49 KB (7,548 words) - 15:38, 9 May 2012
- ** [[Selecting Spectral Windows and Channels]] [http://www.splatalogue.net Splatalogue - Astronomical Line Database]6 KB (845 words) - 11:21, 18 July 2017
- ...c corrections. These VLA standard calibrators, however, exhibit a negative spectral index and are relatively weak at high frequencies. ...error in the bandpass calibration. This tutorial describes how to model a spectral slope and how to correct the bandpass solution for this effect.28 KB (3,769 words) - 11:37, 10 July 2019
- ...c corrections. These VLA standard calibrators, however, exhibit a negative spectral index and are relatively weak at high frequencies. ...error in the bandpass calibration. This tutorial describes how to model a spectral slope and how to correct the bandpass solution for this effect.28 KB (3,783 words) - 13:04, 13 November 2020
- ...c corrections. These VLA standard calibrators, however, exhibit a negative spectral index and are relatively weak at high frequencies. ...error in the bandpass calibration. This tutorial describes how to model a spectral slope and how to correct the bandpass solution for this effect.26 KB (3,524 words) - 10:41, 14 June 2016
- ...c corrections. These VLA standard calibrators, however, exhibit a negative spectral index and are relatively weak at high frequencies. ...error in the bandpass calibration. This tutorial describes how to model a spectral slope and how to correct the bandpass solution for this effect.26 KB (3,524 words) - 13:14, 20 April 2017
- ...c corrections. These VLA standard calibrators, however, exhibit a negative spectral index and are relatively weak at high frequencies. ...error in the bandpass calibration. This tutorial describes how to model a spectral slope and how to correct the bandpass solution for this effect.26 KB (3,524 words) - 11:47, 18 November 2016
- ...c corrections. These VLA standard calibrators, however, exhibit a negative spectral index and are relatively weak at high frequencies. ...error in the bandpass calibration. This tutorial describes how to model a spectral slope and how to correct the bandpass solution for this effect.29 KB (3,922 words) - 11:40, 2 May 2022
