Caltech CASA Tutorials: Difference between revisions
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* EVLA: [http://casaguides.nrao.edu/index.php?title=EVLA_high_frequency_Spectral_Line_tutorial_-_IRC%2B10216_part1_%28Caltech%29 IRC+10216 -- Spectral line, Ka-band (36 GHz)] | * EVLA: [http://casaguides.nrao.edu/index.php?title=EVLA_high_frequency_Spectral_Line_tutorial_-_IRC%2B10216_part1_%28Caltech%29 IRC+10216 -- Spectral line, Ka-band (36 GHz)] | ||
<blockquote> | |||
Calibrate and make image cubes of the line emission from this asymptotic giant branch star. This is a high-frequency EVLA dataset. Includes: | |||
* Inspecting data; basic flagging & calibration | |||
* Subtracting continuum emission | |||
* Imaging the spectral lines | |||
* Imaging the continuum | |||
* Image analysis | |||
* Self-calibration | |||
</blockquote> | |||
* EVLA: [http://casaguides.nrao.edu/index.php?title=EVLA_Wide-Band_Wide-Field_Imaging:_G55.7_3.4_%28Caltech%29 G55.7+3.4 -- Wide-band, wide-field imaging; L-band (1-2 GHz)] | * EVLA: [http://casaguides.nrao.edu/index.php?title=EVLA_Wide-Band_Wide-Field_Imaging:_G55.7_3.4_%28Caltech%29 G55.7+3.4 -- Wide-band, wide-field imaging; L-band (1-2 GHz)] | ||
* ALMA: [http://casaguides.nrao.edu/index.php?title=TWHydraBand7_(Caltech) TW Hydra -- Spectral line, Band 7 (650 micron)] | * ALMA: [http://casaguides.nrao.edu/index.php?title=TWHydraBand7_(Caltech) TW Hydra -- Spectral line, Band 7 (650 micron)] |
Revision as of 20:54, 13 January 2012
Tutorials for the Caltech CASA Radio Analysis Workshop:
Calibrate and image a galaxy field for this mid-frequency EVLA observation. This includes:
- Excising RFI from the data
- Basic flagging and calibration steps
- Imaging from one spectral window to full dataset
- Using multi-scale, multi-frequency synthesis
- Image analysis
Calibrate and make image cubes of the line emission from this asymptotic giant branch star. This is a high-frequency EVLA dataset. Includes:
- Inspecting data; basic flagging & calibration
- Subtracting continuum emission
- Imaging the spectral lines
- Imaging the continuum
- Image analysis
- Self-calibration