CARMA Tutorials: Difference between revisions

From CASA Guides
Jump to navigationJump to search
No edit summary
No edit summary
Line 1: Line 1:
* Reducing a Spectral-Line mosaic (using CO J=1-0 in NGC4254 from CARMA STING, Rahman et al. 2010)
Reducing a Spectral-Line mosaic (using CO J=1-0 in M99 (NGC4254) from CARMA STING, Rahman et al. 2010)
** [[Extracting data from MIRIAD]]
We present two methods:
** Before you calibrate: try [[Data flagging with plotms]] or [[Data flagging with viewer]]. (These demonstrate flagging with VLA data, but are quite thorough and well worth a look.)
Using the wideband to calibrate the narrowbands:
** [[Importing and Calibrating a Mosaicked Spectral Line Dataset]]
* [[CARMA spectral line mosaic M99]] (developed for the 2010 NRAO Synthesis Summer School)
** [[Imaging a Mosaicked Spectral Line Dataset]]
Calibrating each spectral window separately (only for very strong phase calibrators):
* [[Extracting data from MIRIAD]]
* [[Importing and Calibrating a Mosaicked Spectral Line Dataset]]
* [[Imaging a Mosaicked Spectral Line Dataset]]

Revision as of 14:13, 17 May 2010

Reducing a Spectral-Line mosaic (using CO J=1-0 in M99 (NGC4254) from CARMA STING, Rahman et al. 2010) We present two methods: Using the wideband to calibrate the narrowbands:

Calibrating each spectral window separately (only for very strong phase calibrators):