Past MM/Submm Guides: Difference between revisions
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Created page with "Below is a listing of older millimeter/submillimeter casaguides that may be of interest to users: * EVLA Ka-Band (36 GHz/10 mm) Spectral Line Observations of the AGB Star ([h..." |
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Here are several older millimeter/submillimeter casaguides that may be of interest to users. Note that they are not currently being maintained and have been last validated for the CASA version listed beside each. | |||
For CASA guides that focus on VLA data, please see [[Karl_G._Jansky_VLA_Tutorials | Karl G. Jansky VLA Tutorials.]] | |||
* Reducing a CARMA Spectral-Line mosaic of CO(1-0) in M99 (NGC4254) from the STING collaboration (Rahman et al. 2010) using the a wideband spectral window to calibrate the narrowband spectral windows | * [[CARMA spectral line mosaic M99]]: Reducing a CARMA Spectral-Line mosaic of CO(1-0) in M99 (NGC4254) from the STING collaboration (Rahman et al. 2010) using the a wideband spectral window to calibrate the narrowband spectral windows. Last checked in CASA 3.1. | ||
* [[SMA CO Line Data_3.2 | SMA CO Line Data]]: SMA Mosaic Observation of an Infrared Dark Cloud in CO(2-1). Last checked in CASA 3.2. | |||
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* EVLA Ka-Band (36 GHz/10 mm) Spectral Line Observations of the AGB Star ([http://simbad.u-strasbg.fr/simbad/sim-id?Ident=CW+Leo&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id IRC +10216]) | |||
** Data Calibration: [[EVLA Spectral Line Calibration IRC+10216]] | |||
** Data Imaging and Analysis: [[EVLA Spectral Line Imaging Analysis IRC+10216]] | |||
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Latest revision as of 14:20, 18 November 2024
Here are several older millimeter/submillimeter casaguides that may be of interest to users. Note that they are not currently being maintained and have been last validated for the CASA version listed beside each.
For CASA guides that focus on VLA data, please see Karl G. Jansky VLA Tutorials.
- CARMA spectral line mosaic M99: Reducing a CARMA Spectral-Line mosaic of CO(1-0) in M99 (NGC4254) from the STING collaboration (Rahman et al. 2010) using the a wideband spectral window to calibrate the narrowband spectral windows. Last checked in CASA 3.1.
- SMA CO Line Data: SMA Mosaic Observation of an Infrared Dark Cloud in CO(2-1). Last checked in CASA 3.2.
