Current MM/Submm Guides: Difference between revisions
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Below is a listing of current millmeter/submillimeter casaguides that may be of interest to future ALMA users | Below is a listing of current millmeter/submillimeter casaguides that may be of interest to future ALMA users | ||
* EVLA Ka-Band (36 GHz) 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]) | * 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 Calibration: [[EVLA Spectral Line Calibration IRC+10216]] | ||
** Data Imaging and Analysis: [[EVLA Spectral Line Imaging Analysis IRC+10216]] | ** Data Imaging and Analysis: [[EVLA Spectral Line Imaging Analysis IRC+10216]] |
Revision as of 20:01, 9 June 2010
Below is a listing of current millmeter/submillimeter casaguides that may be of interest to future ALMA users
- EVLA Ka-Band (36 GHz/10 mm) Spectral Line Observations of the AGB Star (IRC +10216)
- Data Calibration: EVLA Spectral Line Calibration IRC+10216
- Data Imaging and Analysis: EVLA Spectral Line Imaging Analysis IRC+10216
- 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
- SMA Mosaic Observation of an Infrared Dark Cloud in CO(2-1):SMA CO Line Data